gnuastro-0.5/0000755000175000017500000000000013217220471010220 500000000000000gnuastro-0.5/.tarball-version0000644000175000017500000000000413217220471013237 000000000000000.5 gnuastro-0.5/tests/0000755000175000017500000000000013217220471011362 500000000000000gnuastro-0.5/tests/during-dev.sh0000755000175000017500000001366113216276304013721 00000000000000#! /bin/sh # Script to rebuild and test a utility during development. # # During the development of Gnuastro, you often make changes in a utility # then need to rebuild and run it with special arguments and options (to # test your work). This script is made to facilitate this process. It will # take these steps: # # 1. Delete an existing utility executable. # # 2. Run Make on all Gnuastro. # # 3. If Make was successful, then go into the output directory, and run # utility with the given arguments and options. The executable is run # within an output directory (possibly different from the source or # build directories) so if you need to make lots of temporary test # files, there they won't get mixed up with non-output files. # # Combined with the `tmpfs-config-make', this script can be used to greatly # simplify the development process. After running that script once, for # subsequent builds during your development, you can run this script from # the top source directory (by running `./tests/during-dev.sh', or giving # this to the `compile' command in Emacs). Note that you have to set the # first few variables (directories, utility name, arguments and options) # manually before each major development activity. # # This file will be changed alot during development. So please make sure # you have left the variable values empty before committing. This will # remind each developer running this script to set the values based on # their particular work. Alternatively you can reset this file to its # version controlled status before committing your main work with the # command below: # # git checkout -- tests/during-dev.sh # # This file can also be used as a model to write a test for the work you # have done (to be checked with `make check'). Just copy and paste an # existing test from the utility and replace the last few lines based on # this file. # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it under # the terms of the GNU General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # Gnuastro is distributed in the hope that it will be useful, but WITHOUT # ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or # FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for # more details. # # You should have received a copy of the GNU General Public License along # with Gnuastro. If not, see . # SET INPUT PARAMETERS # ==================== # Set the basic test directories. If you are building over the source # directory, then set `builddir' to `./'. If you want the outputs to be in # the top source directory, set it to `./'. Since 'build' is the assumed # symbolic link in `tmpfs-config-make', it is also assumed in the version # controlled version of this script. Note, if your directory names have # space characters in them, quote the full value numjobs=8 builddir=build outdir= # Set the utility name, along with its arguments and options. NOTE, for # multiple arguments and options, please put them all between quotation # marks so the space characters are included. If there are spaces in the # values of the options or arguments, quote them two times (once for this # script, and once for the utility. In such cases it might be easier to # just add the argument/option to the final script that runs the utility # rather than these variables. utilname= arguments= options= # RUN THE PROCEDURES # ================== # First, make sure the variables are set. Note that arguments and options # are not absolutly vital! so they are not checked here. The utility will # warn and halt if it needs them. if [ x"$outdir" = x ]; then echo "outdir is not set."; exit 1; fi if [ x$utilname = x ]; then echo "utilname is not set."; exit 1; fi if [ x"$numjobs" = x ]; then echo "numjobs is not set."; exit 1; fi if [ x"$builddir" = x ]; then echo "builddir is not set."; exit 1; fi # If builddir is relative, then append the current directory to make it # absolute. This is done because we will be going into the output directory # for executing the utility and we need to know the absolute address of the # top build directory. srcdir=$(pwd) if [ ! "${builddir:0:1}" = "/" ]; then builddir="$srcdir/$builddir" fi # Set the utility's executable file name utility="$builddir/bin/$utilname/ast$utilname" # If the utility is already built, then remove the executable so it is # definitely remade. if [ -f "$utility" ]; then rm "$utility"; fi # Make Gnuastro (note that during development, it is sometimes necessary to # edit/rebuild the libraries too). If Make is successful, then change to # the output directory and run the utility with the given arguments and # options. # # Before actually running put a copy of the configuration file in the # output directory and also add the onlydirconf option so user or system # wide configuration files don't interfere. if make -j$numjobs -C "$builddir"; then # Change to the output directory. cd "$outdir" # Make the .gnuastro directory if it doesn't exist. if [ ! -d .gnuastro ]; then mkdir .gnuastro fi # Put a copy of this utility's configuration file there and add the # onlydirconf option. We are first printing an empty line just in case # the last line in the configuration file doesn't actualy end with a # new line (in which case the appended string will be added to the end # of the last line). cp "$srcdir/bin/gnuastro.conf" "$srcdir/bin/$utilname/ast$utilname.conf" \ .gnuastro/ echo "" >> .gnuastro/gnuastro.conf echo " lastconfig 1" >> .gnuastro/gnuastro.conf # Run the built utility with the given arguments and options. "$utility" $arguments $options # Clean up. rm -rf .gnuastro fi gnuastro-0.5/tests/prepconf.sh0000755000175000017500000000502613216276304013465 00000000000000# This is not actually a test of any of the programs, it just brings # in all the configuration files into a locally created .gnuastro # directory for all the tests to use. It is part of the GNU Astronomy # Utilities (Gnuastro). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # Gnuastro is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with Gnuastro. If not, see . # Make the .gnuastro directory # ---------------------------- # # This directory will keep the default configuration files for all the # programs. If it already exists, delete it. `mkdir_p' is the equivalent to # GNU's `mkdir -p' which might not exist on some systems. It comes from # Autoconf's tests and is exported to the test shell scripts from the # `tests/Makefile.am' file. $mkdir_p .gnuastro # Common options for all programs # ------------------------------- # # Copy the common options while adding the following optios only for make # check. # # - `lastconfig' will make sure that the program stop searching for # configuration files after this one. # # - Log files are not necessary during tests, they are mainly used for # reporting extra information about successful tests. Failed messages # will be printed on the command-line not in a log-file. 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GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ 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dvi \ dvi-am html html-am info info-am install install-am \ install-data install-data-am install-dvi install-dvi-am \ install-exec install-exec-am install-html install-html-am \ install-info install-info-am install-man install-pdf \ install-pdf-am install-ps install-ps-am install-strip \ installcheck installcheck-am installdirs maintainer-clean \ maintainer-clean-generic mostlyclean mostlyclean-compile \ mostlyclean-generic mostlyclean-libtool pdf pdf-am ps ps-am \ recheck tags tags-am uninstall uninstall-am .PRECIOUS: Makefile @COND_ARITHMETIC_TRUE@ arithmetic/onlynumbers.sh: prepconf.sh.log @COND_ARITHMETIC_TRUE@ arithmetic/snimage.sh: noisechisel/noisechisel.sh.log @COND_ARITHMETIC_TRUE@ arithmetic/where.sh: noisechisel/noisechisel.sh.log @COND_ARITHMETIC_TRUE@ arithmetic/or.sh: noisechisel/noisechisel.sh.log @COND_BUILDPROG_TRUE@ buildprog/simpleio.sh: mkprof/mosaic1.sh.log @COND_CONVERTT_TRUE@ convertt/fitstotxt.sh: mkprof/mosaic1.sh.log @COND_CONVERTT_TRUE@ convertt/fitstojpeg.sh: mkprof/mosaic1.sh.log @COND_CONVERTT_TRUE@ convertt/blankch.sh: mkprof/mosaic1.sh.log @COND_CONVERTT_TRUE@ convertt/jpegtotxt.sh: convertt/fitstojpeg.sh.log @COND_CONVERTT_TRUE@ convertt/fitstojpegcmyk.sh: mkprof/mosaic1.sh.log @COND_CONVERTT_TRUE@ convertt/jpegtofits.sh: convertt/blankch.sh.log @COND_CONVERTT_TRUE@ convertt/fitstopdf.sh: crop/section.sh.log @COND_CONVOLVE_TRUE@ convolve/spatial.sh: mkprof/mosaic1.sh.log @COND_CONVOLVE_TRUE@ convolve/frequency.sh: mkprof/mosaic1.sh.log @COND_COSMICCAL_TRUE@ cosmiccal/simpletest.sh: prepconf.sh.log @COND_CROP_TRUE@ crop/imgcat.sh: mkprof/mosaic1.sh.log @COND_CROP_TRUE@ crop/wcscat.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ @COND_CROP_TRUE@ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log @COND_CROP_TRUE@ crop/imgcenter.sh: mkprof/mosaic1.sh.log @COND_CROP_TRUE@ crop/imgcenternoblank.sh: mkprof/mosaic1.sh.log @COND_CROP_TRUE@ crop/section.sh: mkprof/mosaic1.sh.log @COND_CROP_TRUE@ crop/wcscenter.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ @COND_CROP_TRUE@ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log @COND_CROP_TRUE@ crop/imgpolygon.sh: mkprof/mosaic1.sh.log @COND_CROP_TRUE@ crop/imgoutpolygon.sh: mkprof/mosaic1.sh.log @COND_CROP_TRUE@ crop/wcspolygon.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ @COND_CROP_TRUE@ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log @COND_FITS_TRUE@ fits/write.sh: mkprof/mosaic1.sh.log @COND_FITS_TRUE@ fits/print.sh: fits/write.sh.log @COND_FITS_TRUE@ fits/update.sh: fits/write.sh.log @COND_FITS_TRUE@ fits/delete.sh: fits/write.sh.log @COND_FITS_TRUE@ fits/copyhdu.sh: fits/write.sh.log mkprof/mosaic2.sh.log @COND_MATCH_TRUE@ match/positions.sh: prepconf.sh.log @COND_MATCH_TRUE@ match/merged-cols.sh: prepconf.sh.log @COND_MKCATALOG_TRUE@ mkcatalog/simple.sh: noisechisel/noisechisel.sh.log @COND_MKCATALOG_TRUE@ mkcatalog/aperturephot.sh: noisechisel/noisechisel.sh.log \ @COND_MKCATALOG_TRUE@ mkprof/clearcanvas.sh.log @COND_MKNOISE_TRUE@ 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convolve/spatial.sh.log @COND_WARP_TRUE@ warp/homographic.sh: convolve/spatial.sh.log lib/multithread.sh: mkprof/mosaic1.sh.log # CLEANFILES is only for files, not directories. Therefore we are using # Automake's extending rules to clean the temporary `.gnuastro' directory # that was built by the `prepconf.sh' scripot. See "Extending Automake # rules", and the "What Gets Cleaned" sections of the Automake manual. clean-local:; rm -rf .gnuastro # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.5/tests/Makefile.am0000644000175000017500000002165113216276304013350 00000000000000## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Translate conditions that came from `./configure' into variables that can ## be used here. This includes the programs and teh dependencies of the ## checks. ## ## Dependency structure ## ==================== ## ## The tests depend on each other. One way to fix this is to call them in ## the order that their dependence is satisfied. But that is prone to ## errors and a lot of problem. The user also not want to build all the ## programs. Also, Make allows us to work with multiple threads (with ## `-jN') and in that case, it is vital to define the dependencies. ## ## The output of all the tests that should be used (is recognized by ## Automake and will not mess the system) is the name of the test file ## appended by a `.log'. It contains the output of the program on standard ## output and error. THIS IS IMPORTANT: So even if the program fails, the ## .log file is created. The check if the input for a test exists or not ## should be checked in the test that depends on it, it can't be done here ## in the Makefile. if COND_HASGHOSTSCRIPT MAYBE_HASGHOSTSCRIPT = "yes" endif if COND_HASLIBJPEG MAYBE_HASLIBJPEG = "yes" endif if COND_HASGNULIBTOOL MAYBE_HASGNULIBTOOL = "yes" endif if COND_ARITHMETIC MAYBE_ARITHMETIC_TESTS = arithmetic/snimage.sh arithmetic/onlynumbers.sh \ arithmetic/where.sh arithmetic/or.sh arithmetic/onlynumbers.sh: prepconf.sh.log arithmetic/snimage.sh: noisechisel/noisechisel.sh.log arithmetic/where.sh: noisechisel/noisechisel.sh.log arithmetic/or.sh: noisechisel/noisechisel.sh.log endif if COND_BUILDPROG MAYBE_BUILDPROG_TESTS = buildprog/simpleio.sh buildprog/simpleio.sh: mkprof/mosaic1.sh.log endif if COND_CONVERTT MAYBE_CONVERTT_TESTS = convertt/fitstotxt.sh convertt/fitstojpeg.sh \ convertt/blankch.sh convertt/jpegtotxt.sh convertt/fitstojpegcmyk.sh \ convertt/jpegtofits.sh convertt/fitstopdf.sh convertt/fitstotxt.sh: mkprof/mosaic1.sh.log convertt/fitstojpeg.sh: mkprof/mosaic1.sh.log convertt/blankch.sh: mkprof/mosaic1.sh.log convertt/jpegtotxt.sh: convertt/fitstojpeg.sh.log convertt/fitstojpegcmyk.sh: mkprof/mosaic1.sh.log convertt/jpegtofits.sh: convertt/blankch.sh.log convertt/fitstopdf.sh: crop/section.sh.log endif if COND_CONVOLVE MAYBE_CONVOLVE_TESTS = convolve/spatial.sh convolve/frequency.sh convolve/spatial.sh: mkprof/mosaic1.sh.log convolve/frequency.sh: mkprof/mosaic1.sh.log endif if COND_COSMICCAL MAYBE_COSMICCAL_TESTS = cosmiccal/simpletest.sh cosmiccal/simpletest.sh: prepconf.sh.log endif if COND_CROP MAYBE_CROP_TESTS = crop/imgcat.sh crop/wcscat.sh crop/imgcenter.sh \ crop/imgcenternoblank.sh crop/section.sh crop/wcscenter.sh \ crop/imgpolygon.sh crop/imgoutpolygon.sh crop/wcspolygon.sh crop/imgcat.sh: mkprof/mosaic1.sh.log crop/wcscat.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log crop/imgcenter.sh: mkprof/mosaic1.sh.log crop/imgcenternoblank.sh: mkprof/mosaic1.sh.log crop/section.sh: mkprof/mosaic1.sh.log crop/wcscenter.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log crop/imgpolygon.sh: mkprof/mosaic1.sh.log crop/imgoutpolygon.sh: mkprof/mosaic1.sh.log crop/wcspolygon.sh: mkprof/mosaic1.sh.log mkprof/mosaic2.sh.log \ mkprof/mosaic3.sh.log mkprof/mosaic4.sh.log endif if COND_FITS MAYBE_FITS_TESTS = fits/write.sh fits/print.sh fits/update.sh \ fits/delete.sh fits/copyhdu.sh fits/write.sh: mkprof/mosaic1.sh.log fits/print.sh: fits/write.sh.log fits/update.sh: fits/write.sh.log fits/delete.sh: fits/write.sh.log fits/copyhdu.sh: fits/write.sh.log mkprof/mosaic2.sh.log endif if COND_MATCH MAYBE_MATCH_TESTS = match/positions.sh match/merged-cols.sh match/positions.sh: prepconf.sh.log match/merged-cols.sh: prepconf.sh.log endif if COND_MKCATALOG MAYBE_MKCATALOG_TESTS = mkcatalog/simple.sh mkcatalog/aperturephot.sh mkcatalog/simple.sh: noisechisel/noisechisel.sh.log mkcatalog/aperturephot.sh: noisechisel/noisechisel.sh.log \ mkprof/clearcanvas.sh.log endif if COND_MKNOISE MAYBE_MKNOISE_TESTS = mknoise/addnoise.sh mknoise/addnoise.sh: warp/warp_scale.sh.log endif if COND_MKPROF MAYBE_MKPROF_TESTS = mkprof/mosaic1.sh mkprof/mosaic2.sh \ mkprof/mosaic3.sh mkprof/mosaic4.sh mkprof/radeccat.sh \ mkprof/ellipticalmasks.sh mkprof/clearcanvas.sh mkprof/mosaic1.sh: prepconf.sh.log mkprof/mosaic2.sh: prepconf.sh.log mkprof/mosaic3.sh: prepconf.sh.log mkprof/mosaic4.sh: prepconf.sh.log mkprof/radeccat.sh: prepconf.sh.log mkprof/ellipticalmasks.sh: mknoise/addnoise.sh.log mkprof/clearcanvas.sh: mknoise/addnoise.sh.log endif if COND_NOISECHISEL MAYBE_NOISECHISEL_TESTS = noisechisel/noisechisel.sh noisechisel/noisechisel.sh: mknoise/addnoise.sh.log endif if COND_STATISTICS MAYBE_STATISTICS_TESTS = statistics/basicstats.sh statistics/estimate_sky.sh statistics/basicstats.sh: mknoise/addnoise.sh.log statistics/estimate_sky.sh: mknoise/addnoise.sh.log endif if COND_TABLE MAYBE_TABLE_TESTS = table/txt-to-fits-binary.sh \ table/fits-binary-to-txt.sh table/txt-to-fits-ascii.sh \ table/fits-ascii-to-txt.sh table/txt-to-fits-binary.sh: prepconf.sh.log table/fits-binary-to-txt.sh: table/txt-to-fits-binary.sh.log table/txt-to-fits-ascii.sh: prepconf.sh.log table/fits-ascii-to-txt.sh: table/txt-to-fits-ascii.sh.log endif if COND_WARP MAYBE_WARP_TESTS = warp/warp_scale.sh warp/homographic.sh warp/warp_scale.sh: convolve/spatial.sh.log warp/homographic.sh: convolve/spatial.sh.log endif # `config.h' is built by `../lib/Makefile.am' and is only meant for outside # users (internally `config.h' has everything). Thus, we need to add it to # the include directories of the test programs in this directory. AM_CPPFLAGS = -I../lib # Environment variables for the test scripts. AM_TESTS_ENVIRONMENT = \ export mkdir_p="$(MKDIR_P)"; \ export topsrc=$(top_srcdir); \ export haslibjpeg=$(MAYBE_HASLIBJPEG); \ export hasgnulibtool=$(MAYBE_HASGNULIBTOOL); \ export hasghostscript=$(MAYBE_HASGHOSTSCRIPT); # Library checks # ============== # # The Gnuastro library is checked by compiling programs and linking them # with the library. As described in the last paragraph of the "Scripts # based test suites" section of the Automake manual, all targets specified # by `check_PROGRAMS' are compiled prior to actually running the targets of # `TESTS'. So they do not need to be specified as any dependency, they will # be present when the `.sh' based tests are run. LDADD = -lgnuastro check_PROGRAMS = multithread versioncxx multithread_SOURCES = lib/multithread.c versioncxx_SOURCES = lib/versioncxx.cpp lib/multithread.sh: mkprof/mosaic1.sh.log # Final Tests # =========== TESTS = prepconf.sh lib/multithread.sh lib/versioncxx.sh \ $(MAYBE_ARITHMETIC_TESTS) $(MAYBE_BUILDPROG_TESTS) \ $(MAYBE_CONVERTT_TESTS) $(MAYBE_CONVOLVE_TESTS) $(MAYBE_COSMICCAL_TESTS) \ $(MAYBE_CROP_TESTS) $(MAYBE_FITS_TESTS) $(MAYBE_MATCH_TESTS) \ $(MAYBE_MKCATALOG_TESTS) $(MAYBE_MKNOISE_TESTS) $(MAYBE_MKPROF_TESTS) \ $(MAYBE_NOISECHISEL_TESTS) $(MAYBE_STATISTICS_TESTS) \ $(MAYBE_SUBTRACTSKY_TESTS) $(MAYBE_TABLE_TESTS) $(MAYBE_WARP_TESTS) # Files to distribute along with the tests. EXTRA_DIST = $(TESTS) during-dev.sh buildprog/simpleio.c crop/cat.txt \ match/positions-1.txt match/positions-2.txt mkprof/mkprofcat1.txt \ mkprof/ellipticalmasks.txt mkprof/clearcanvas.txt mkprof/mkprofcat2.txt \ mkprof/mkprofcat3.txt mkprof/mkprofcat4.txt mkprof/radeccat.txt \ table/table.txt # Files that must be cleaned with `make clean'. CLEANFILES = *.log *.txt *.jpg *.fits *.pdf *.eps simpleio # CLEANFILES is only for files, not directories. Therefore we are using # Automake's extending rules to clean the temporary `.gnuastro' directory # that was built by the `prepconf.sh' scripot. See "Extending Automake # rules", and the "What Gets Cleaned" sections of the Automake manual. clean-local:; rm -rf .gnuastro gnuastro-0.5/tests/warp/0000755000175000017500000000000013217220471012333 500000000000000gnuastro-0.5/tests/warp/homographic.sh0000755000175000017500000000262513121462410015112 00000000000000# Apply a general homographic transformation to an image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=warp img=convolve_spatial.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --output=homographic.fits \ --matrix="0.707106781,-0.707106781,0, 0.707106781, 0.707106781,0, 0.001,0.002,1" --coveredfrac=0.5 gnuastro-0.5/tests/warp/warp_scale.sh0000755000175000017500000000243313121462410014727 00000000000000# Scale an image to 1/5th of its input scale. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=warp img=convolve_spatial.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --scale=1/5 --centeroncorner gnuastro-0.5/tests/table/0000755000175000017500000000000013217220471012451 500000000000000gnuastro-0.5/tests/table/table.txt0000644000175000017500000000510613121462410014216 00000000000000# A single table to test the reading and writing functions. # # - It contains all the types. # - String columns, names, and units have space characters. # - Blank values in all the columns. # - Empty lines (not comment or data. # - Column information comments are not in the same order as data. # - A column with no information. # - Columns with missing information # - Some blank values different from the internal blank values. # Column 10: DOUBLE [no units, f64, 255] Column with double values # Column 1: UINT8_DATA [no units, u8, 5] Column with unsigned char values # Column 2: INT8 [no-units, i8] Column with char values # Column 3: STRING data [, str21, no data] Column with string values # Column 4: UINT16 data [,u16] Column with unsigned short values # Column 5: INT16 [no units, i16] Column with short values # Column 7: INT32 [no units, i32] Column with long values # Column 8: INT64 [no units, i64] Another column of long values # Column 9: FLOAT32 [no units, f32,-99] Column with float values # Column 6: UINT32 [,u32] # IMPORTANT NOTE FOR FITS ASCII tables: CFITSIO will give its error # 412 (data type conversion overflow) when the number cannot be # printed in the provided space (with full precision). So make sure # that the full-integer part of the number has less characters than # the `width - precision - 1' (when everything is default, you can get # these values from `lib/gnuastro/table.h'). 1 -1 The vertical lines 3455 -3455 1 -1 9 1874.103872 8.391334343995 1 2 -2 are only for easy 3466 -3466 2 -2 10 123.93373 893.3497e5 2 3 -3 visual identification 3467 -3467 3 -3 12 -0.737648 nan 3 4 -4 of the limits of this 3468 -3468 4 -4 800 78.983 8.2328438e8 4 5 -5 |string column. | 3469 -3469 5 -5 8923 -99 -7.32384e4 5 6 -6 |characters beyond | 20821 -20821 6 -6 9823 -99 nan 6 7 -7 the last one will be 20822 -20822 7 -7 7232 9999 8.3343e-5 7 8 -8 read as a number. 20823 -20823 8 -8 921 2.3 934892734.82 8 9 -9 With@Some#!STRANGE@ 60983 -25722 9 -9 8127 -99 3474924.489252 9 10 -10 Characters%^&*()~ 62182 -30100 10 -10 8287 7.3e-4 -3467.3432e5 10 11 -12 no data 65500 -32700 11 -11 999 8.73E2 nan 11 255 -12 -- Last Line :-) -- 65501 -32701 12 -12 8282 892.23 8975.3653 12 gnuastro-0.5/tests/table/fits-ascii-to-txt.sh0000755000175000017500000000243113121462410016213 00000000000000# Convert an ASCII table to a binary table # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=table table=ascii-table.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $table ]; then echo "$table doesn't exist."; exit 77; fi # Actual test script # ================== $execname $table --output=from-ascii-table.txt gnuastro-0.5/tests/table/txt-to-fits-ascii.sh0000755000175000017500000000247313121462410016221 00000000000000# Convert an ASCII table to a binary table # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=table execname=../bin/$prog/ast$prog table=$topsrc/tests/$prog/table.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $table ]; then echo "$table doesn't exist."; exit 77; fi # Actual test script # ================== $execname $table --output=ascii-table.fits --tableformat=fits-ascii gnuastro-0.5/tests/table/fits-binary-to-txt.sh0000755000175000017500000000243313121462410016411 00000000000000# Convert an ASCII table to a binary table # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=table table=binary-table.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $table ]; then echo "$table doesn't exist."; exit 77; fi # Actual test script # ================== $execname $table --output=from-binary-table.txt gnuastro-0.5/tests/table/txt-to-fits-binary.sh0000755000175000017500000000247513121462410016417 00000000000000# Convert an ASCII table to a binary table # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=table execname=../bin/$prog/ast$prog table=$topsrc/tests/$prog/table.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $table ]; then echo "$table does not exist."; exit 77; fi # Actual test script # ================== $execname $table --output=binary-table.fits --tableformat=fits-binary gnuastro-0.5/tests/statistics/0000755000175000017500000000000013217220471013554 500000000000000gnuastro-0.5/tests/statistics/estimate_sky.sh0000755000175000017500000000300313121462410016523 00000000000000# Estimate the Sky value on input image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=statistics execname=../bin/$prog/ast$prog img=convolve_spatial_noised.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== # # Note that to keep things simple we are not convolving the image, so the # result will not be too accurate! Here we just want to see if the full # tessellation, estimation, interpolation and smoothing go nicely without # any errors. $execname $img --sky --checksky gnuastro-0.5/tests/statistics/basicstats.sh0000755000175000017500000000244313121462410016171 00000000000000# Get basic image statistics. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=statistics execname=../bin/$prog/ast$prog img=convolve_spatial_scaled_noised.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img -g9500 -l11000 --numasciibins=65 gnuastro-0.5/tests/noisechisel/0000755000175000017500000000000013217220471013667 500000000000000gnuastro-0.5/tests/noisechisel/noisechisel.sh0000755000175000017500000000260313156610402016453 00000000000000# Detect objects and clumps in an image using NoiseChisel. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=noisechisel execname=../bin/$prog/ast$prog img=convolve_spatial_noised.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --cleangrowndet --checkdetection --checksegmentation \ --continueaftercheck --tilesize=100,100 gnuastro-0.5/tests/mkprof/0000755000175000017500000000000013217220471012660 500000000000000gnuastro-0.5/tests/mkprof/radeccat.txt0000644000175000017500000000172513121462410015107 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: RA [deg, f64] Right Ascension of profile center # Column 3: Dec [deg, f64] Declination of profile center # Column 4: Function [name, str7] Profile's radial function # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile 1 0.99987331 1.0001617 sersic 10.00 2.500 45.000 0.3 -6.0 2.000 2 0.99929656 1.0006917 sersic 10.00 2.500 135.00 0.3 -6.0 2.000 gnuastro-0.5/tests/mkprof/mkprofcat4.txt0000644000175000017500000000153413121462410015411 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: X [pixel, f64] X axis position of profile center # Column 3: Y [pixel, f64] Y axis position of profile center # Column 4: Function [name, str7] Profile's radial function # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile 1 0.40 0.40 sersic 20.00 2.500 45.000 1.00 -18.0 5.000 gnuastro-0.5/tests/mkprof/mkprofcat3.txt0000644000175000017500000000153613121462410015412 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: X [pixel, f64] X axis position of profile center # Column 3: Y [pixel, f64] Y axis position of profile center # Column 4: Function [code, i32] Profile's radial function code # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile 1 100.40 0.40 1 20.00 2.500 45.000 1.00 -18.0 5.000 gnuastro-0.5/tests/mkprof/mkprofcat2.txt0000644000175000017500000000153713121462410015412 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: X [pixel, f64] X axis position of profile center # Column 3: Y [pixel, f64] Y axis position of profile center # Column 4: Function [code, i32] Profile's radial function code # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile 1 0.400 100.40 1 20.00 2.500 45.000 1.00 -18.0 5.000 gnuastro-0.5/tests/mkprof/clearcanvas.txt0000644000175000017500000000177613121462410015631 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: X [pixel, f64] X axis position of profile center # Column 3: Y [pixel, f64] Y axis position of profile center # Column 4: Function [name, str4] Profile's radial function # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile # # Note that the positions and radii are multiplied by 5 compared to `mkprofcat1.txt', # because we are using the over-sampled image as a canvas. # 1 502 502 flat 100 1 45.000 1.000 1 2.000 2 251.605 254.135 flat 29.89 1 77.650 0.801 2 2.000 gnuastro-0.5/tests/mkprof/ellipticalmasks.txt0000644000175000017500000000167213121462410016523 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: X [pixel, f64] X axis position of profile center # Column 3: Y [pixel, f64] Y axis position of profile center # Column 4: Function [name, str7] Profile's radial function # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile 1 100.40 100.40 circum 20.00 2.500 45.000 1.000 NaN 2.000 2 50.321 50.827 flat 5.978 1.320 77.650 0.801 -1 2.000 gnuastro-0.5/tests/mkprof/mkprofcat1.txt0000644000175000017500000000204513121462410015404 00000000000000# Column 1: ID [count, u8] Object ID # Column 2: X [pixel, f64] X axis position of profile center # Column 3: Y [pixel, f64] Y axis position of profile center # Column 4: Function [name, str7] Profile's radial function # Column 5: Width [pixel, f64] For Sersic: effective radius, for Moffat, FWHM # Column 6: Sersic index [none, f64] Sersic index, or Moffat beta # Column 7: Position angle [deg, f64] Position angle of profile # Column 8: Axis ratio [frac, f64] Axis ratio of profile # Column 9: Magnitude [ABmag, f64] Magnitude of profile within truncation radius # Column 10: Truncation radius [dist, f64] Truncation radius to stop building profile 1 0.0000 0.0000 moffat 3.000 4.765 0.0000 1.000 0.000 5.000 2 100.40 100.40 sersic 20.00 2.500 45.000 1.000 -18.0 5.000 3 50.321 50.827 sersic 5.978 1.320 77.650 0.801 -15.0 5.000 gnuastro-0.5/tests/mkprof/clearcanvas.sh0000755000175000017500000000303613121462410015416 00000000000000# Make labeled regions on an image with blank pixels. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog img=convolve_spatial_noised.fits cat=$topsrc/tests/$prog/clearcanvas.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --background=$img --mforflatpix --clearcanvas \ --type=int32 --output="clearcanvas.fits" gnuastro-0.5/tests/mkprof/ellipticalmasks.sh0000755000175000017500000000305713121462410016320 00000000000000# Make two masks (one flat and one circumference) cat1.txt # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog img=convolve_spatial_scaled_noised.fits cat=$topsrc/tests/$prog/ellipticalmasks.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --background=$img --mforflatpix --replace --oversample=1 \ --output="ellipticalmasks.fits" gnuastro-0.5/tests/mkprof/radeccat.sh0000755000175000017500000000241513126521442014710 00000000000000# Create a mock image from radeccat.txt # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/radeccat.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --ccol=RA --ccol=Dec --mode=wcs --naxis=100,100 gnuastro-0.5/tests/mkprof/mosaic4.sh0000755000175000017500000000264213126521442014503 00000000000000# Create a mock image from cat2.txt: # # - It doesn't have any random profiles, only the large profile from # cat1.txt. The central position is set to be on the same real # place as in cat1.txt # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat4.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --naxis=100,100 --crpix=-99,-99 gnuastro-0.5/tests/mkprof/mosaic3.sh0000755000175000017500000000263613126521442014505 00000000000000# Create a mock image from cat2.txt: # # - It doesn't have any random profiles, only the large profile from # cat1.txt. The central position is set to be on the same real # place as in cat1.txt # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat3.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option) # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --naxis=100,100 --crpix=1,-99 gnuastro-0.5/tests/mkprof/mosaic2.sh0000755000175000017500000000273313126521442014502 00000000000000# Create a mock image from cat2.txt: # # - It doesn't have any random profiles, only the large profile from # cat1.txt. The central position is set to be on the same real # place as in cat1.txt # # - Also here, test the individual option. # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat2.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --naxis=100,100 --crpix=-99,1 --individual gnuastro-0.5/tests/mkprof/mosaic1.sh0000755000175000017500000000267413126521442014505 00000000000000# Create a mock image from cat1.txt: # # - It includes one large and bright profile that is on the last # pixel of this image. The other tests will also build the same # profile with the absolute place fixed. # # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkprof execname=../bin/$prog/ast$prog cat=$topsrc/tests/$prog/mkprofcat1.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). # # - Catalog doesn't exist (problem in tarball release). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $cat ]; then echo "$cat does not exist."; exit 77; fi # Actual test script # ================== $execname $cat --naxis=100,100 mv 0_mkprofcat1.fits psf.fits gnuastro-0.5/tests/mknoise/0000755000175000017500000000000013217220471013027 500000000000000gnuastro-0.5/tests/mknoise/addnoise.sh0000755000175000017500000000337313136632404015105 00000000000000# Add noise to an input image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). # # We will be adding noise to two images: the warped (smaller) and unwarped # (larger) mock images. The warped one will be used by programs that don't # care about the size of the image, but the larger one will be used by # those that do: for example SubtractSky and NoiseChisel will be better # tested on a larger image. prog=mknoise img1=convolve_spatial.fits execname=../bin/$prog/ast$prog img2=convolve_spatial_scaled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname doesn't exist."; exit 77; fi if [ ! -f $img1 ]; then echo "$img1 does not exist."; exit 77; fi if [ ! -f $img2 ]; then echo "$img2 does not exist."; exit 77; fi # Actual test script # ================== export GSL_RNG_SEED=1 export GSL_RNG_TYPE=ranlxs2 $execname --envseed $img1 $execname --envseed $img2 gnuastro-0.5/tests/mkcatalog/0000755000175000017500000000000013217220471013324 500000000000000gnuastro-0.5/tests/mkcatalog/aperturephot.sh0000755000175000017500000000301313175442274016334 00000000000000# Make a simple catalog for NoiseChisel's output. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkcatalog objimg=clearcanvas.fits execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi if [ ! -f $objimg ]; then echo "$objimg does not exist"; exit 77; fi # Actual test script # ================== $execname $img --objectsfile=$objimg --objectshdu=1 \ --output=aperturephot.fits \ --objid --x --y --ra --dec --magnitude --sn gnuastro-0.5/tests/mkcatalog/simple.sh0000755000175000017500000000255113121462410015072 00000000000000# Make a simple catalog for NoiseChisel's output. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=mkcatalog execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --x --y --ra --dec --magnitude --upperlimitmag --sn \ --tableformat=txt gnuastro-0.5/tests/match/0000755000175000017500000000000013217220471012456 500000000000000gnuastro-0.5/tests/match/positions-2.txt0000644000175000017500000000025413211616535015332 00000000000000# Column 1: ABCD # Column 2: ACCU1 # Column 3: ACCU2 1 8.20 7.90 2 20.1 2.80 3 4.80 5.20 4 5.01 4.99 5 0.01 0.02 6 6.10 6.05 7 0.99 1.10 gnuastro-0.5/tests/match/positions-1.txt0000644000175000017500000000021513211616535015326 00000000000000# Column 1: ABCD # Column 2: EFGH # Column 3: IJKL 1 1 1 2 2 2 3 3 3 4 4 4 5 5 5 6 6 6 7 7 7 8 8 8 9 9 9 gnuastro-0.5/tests/match/merged-cols.sh0000755000175000017500000000257713211616535015155 00000000000000# Match the two input catalogs and return merged output # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=match execname=../bin/$prog/ast$prog cat1=$topsrc/tests/$prog/positions-1.txt cat2=$topsrc/tests/$prog/positions-2.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi # Actual test script # ================== $execname $cat1 $cat2 --aperture=0.5 --log --output=match-positions.fits \ --outcols=a1,aEFGH,bACCU1,aIJKL,bACCU2 -omatch-merged-cols.txt gnuastro-0.5/tests/match/positions.sh0000755000175000017500000000243313211076737014776 00000000000000# Match the two input catalogs # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=match execname=../bin/$prog/ast$prog cat1=$topsrc/tests/$prog/positions-1.txt cat2=$topsrc/tests/$prog/positions-2.txt # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi # Actual test script # ================== $execname $cat1 $cat2 --aperture=0.5 --log --output=match-positions.fits gnuastro-0.5/tests/lib/0000755000175000017500000000000013217220471012130 500000000000000gnuastro-0.5/tests/lib/versioncxx.sh0000755000175000017500000000176413215601241014623 00000000000000# Run the program to build a report the Gnuastro version in C++. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). execname=./versioncxx # Skip? # ===== # # If the actual executable wasn't built, then this is a hard error and must # be FAIL. if [ ! -f $execname ]; then echo "$execname library program not compiled."; exit 99; fi; # Actual test script # ================== $execname gnuastro-0.5/tests/lib/multithread.sh0000755000175000017500000000234313121462410014726 00000000000000# Run the program to test reading a FITS file to memory and writing it on # the command-line in multi-threaded mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits execname=./multithread # SKIP or FAIL? # ============= # # If the actual executable wasn't built, then this is a hard error and must # be FAIL. But if the input doesn't exist, its not this test's fault. So # just SKIP this test. if [ ! -f $execname ]; then echo "$execname library program not compiled."; exit 99; fi; if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi; # Actual test script # ================== $execname gnuastro-0.5/tests/lib/versioncxx.cpp0000644000175000017500000000215713215601241014765 00000000000000/********************************************************************* A test program to get and use the version number of Gnuastro within C++. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include int main(void) { std::cout << "Gnuastro version is: " << GAL_CONFIG_VERSION << ".\n"; return EXIT_SUCCESS; } gnuastro-0.5/tests/lib/multithread.c0000644000175000017500000000743113164537456014562 00000000000000/********************************************************************* A test program to multithreaded building using Gnuastro's helpers. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include "gnuastro/fits.h" #include "gnuastro/threads.h" /* This structure can keep all information you want to pass onto the worker function on each thread. */ struct params { gal_data_t *image; /* Dataset to print values of. */ }; /* This is the main worker function which will be called by the different threads. `gal_threads_params' is defined in `gnuastro/threads.h' and contains the pointer to the paramter we want. Note that its input and output must have `void *' types. */ void * worker_on_thread(void *in_prm) { /* Low-level definitions to be done first. */ struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct params *p=(struct params *)tprm->params; /* Subsequent definitions. */ float *array=p->image->array; size_t i, index, *dsize=p->image->dsize; /* Go over all the pixels that were assigned to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* For easy reading. */ index = tprm->indexs[i]; /* Print the information. */ printf("(%zu, %zu) on thread %zu: %g\n", index%dsize[1]+1, index/dsize[1]+1, tprm->id, array[index]); } /* Wait for all the other threads to finish, then return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* A simple program to open a FITS image, distributes its pixels between different threads and print the value of each pixel and the thread it was assigned to, this will test both the opening of a FITS file and also the multi-threaded functions. After running `make check' you can see the outputs in `tests/multithread.log'. Please run the following command for an explanation on easily linking and compiling C programs that use Gnuastro's libraries (without having to worry about the libraries to link to) anywhere on your system: $ info gnuastro "Automatic linking script" */ int main(void) { struct params p; char *filename="psf.fits", *hdu="1"; size_t numthreads=gal_threads_number(); /* Read the image into memory as a float32 data type. */ p.image=gal_fits_img_read_to_type(filename, hdu, GAL_TYPE_FLOAT32, -1,0,0); /* Print some basic information before the actual contents: */ printf("Pixel values of %s (HDU: %s) on %zu threads.\n", filename, hdu, numthreads); printf("Used to check the compiled library's capability in opening a " "FITS file, and also spinning-off threads.\n"); /* A small sanity check: this is only intended for 2D arrays. */ if(p.image->ndim!=2) { fprintf(stderr, "only 2D images are supported."); exit(EXIT_FAILURE); } /* Spin-off the threads and do the processing on each thread. */ gal_threads_spin_off(worker_on_thread, &p, p.image->size, numthreads); /* Clean up and return. */ gal_data_free(p.image); return EXIT_SUCCESS; } gnuastro-0.5/tests/fits/0000755000175000017500000000000013217220471012327 500000000000000gnuastro-0.5/tests/fits/copyhdu.sh0000755000175000017500000000257213121462410014262 00000000000000# Copy an extension from one file to another. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=fits img1=fitstest.fits img2=mkprofcat2.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img1 ]; then echo "$img1 does not exist."; exit 77; fi if [ ! -f $img2 ]; then echo "$img2 does not exist."; exit 77; fi # Actual test script # ================== $execname $img2 --copy="Mock profiles" --output=$img1 gnuastro-0.5/tests/fits/delete.sh0000755000175000017500000000240713121462410014046 00000000000000# Delete header information. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=fits img=fitstest.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --delete=ABSJUNK --delete=ABSJNK2 gnuastro-0.5/tests/fits/update.sh0000755000175000017500000000252713121462410014071 00000000000000# Update the full header information # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=fits img=fitstest.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --update=ABSJUNK,8.231,"An updated value.",s \ --update=ABSJNK2,1232,"Another updated value",kg gnuastro-0.5/tests/fits/print.sh0000755000175000017500000000235413121462410013741 00000000000000# Print the full header information # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=fits img=fitstest.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img gnuastro-0.5/tests/fits/write.sh0000755000175000017500000000261113121462410013733 00000000000000# Write a junk header to a FITS file # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=fits img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== cp $img fitstest.fits $execname fitstest.fits --write=ABSJUNK,10.92,"A Fits keyword Test.",m/s \ --date --write=ABSJNK2,2343fdsa,"Another absolute junk test!" gnuastro-0.5/tests/crop/0000755000175000017500000000000013217220471012325 500000000000000gnuastro-0.5/tests/crop/cat.txt0000644000175000017500000000055413121462410013554 00000000000000# Column 1: NAME [name,str4] Name of object. # Column 2: X_CENTER [pixels,f64] Image X axis position. # Column 3: Y_CENTER [pixels,f64] Image Y axis position. # Column 4: RA_CENTER [deg,f64] Right Ascension. # Column 5: DEC_CENTER [deg,f64] Declination. A0B1 500.00 500.00 0.99917157 1.0008283 c2d3 251.00 251.00 0.99958658 1.0004150 gnuastro-0.5/tests/crop/wcspolygon.sh0000755000175000017500000000264613121462410015013 00000000000000# Crop from a catalog using x and y coordinates in WCS mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat*.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi for fn in $img; do if [ ! -f $fn ]; then echo "$fn doesn't exist."; exit 77; fi; done # Actual test script # ================== $execname $img --mode=wcs --zeroisnotblank --output=wcspolygon.fits \ --polygon=0.99980497,1.0001967:0.998378,1.0012267:0.9999766,1.0013217 gnuastro-0.5/tests/crop/imgoutpolygon.sh0000755000175000017500000000314013121462410015511 00000000000000# Crop an image based polygon from an image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img $cat --mode=img --zeroisnotblank --outpolygon \ --polygon=209,50:436.76,151:475.64,438.2:210.6,454.04:121.4,289.88 \ --output=imgoutpolygon.fits gnuastro-0.5/tests/crop/imgpolygon.sh0000755000175000017500000000260513121462410014766 00000000000000# Crop an image based polygon from an image. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img $cat --mode=img --zeroisnotblank --output=imgpolygon.fits \ --polygon=209,50:436.76,151:475.64,438.2:210.6,454.04:121.4,289.88 gnuastro-0.5/tests/crop/wcscenter.sh0000755000175000017500000000256013125235120014577 00000000000000# Crop a box based on center in WCS coordinates. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat*.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi for fn in $img; do if [ ! -f $fn ]; then echo "$fn does not exist."; exit 77; fi; done # Actual test script # ================== $execname $img --center=0.99917157,1.0008283 --output=crop_wcscenter.fits \ --mode=wcs --width=0.3/3600 gnuastro-0.5/tests/crop/section.sh0000755000175000017500000000277713125235120014260 00000000000000# Crop a box based on a specified section. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img --section=-10:*+10,:250 --output=crop_section.fits \ --numthreads=1 --mode=img gnuastro-0.5/tests/crop/imgcenternoblank.sh0000755000175000017500000000311613125235120016122 00000000000000# Crop a region defined by its center in image coordinates, with no blank # pixels. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img --center=500,500 --noblank --numthreads=1 \ --output=crop_imgcenternoblank.fits --mode=img --width=201 gnuastro-0.5/tests/crop/imgcenter.sh0000755000175000017500000000302713125235120014556 00000000000000# Make a single crop with center defined in Image mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. $execname $img --center=251,251 --output=crop_imgcenter.fits \ --numthreads=1 --mode=img --width=201 gnuastro-0.5/tests/crop/wcscat.sh0000755000175000017500000000322113124521666014075 00000000000000# Crop from a catalog using x and y coordinates in WCS mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat*.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi for fn in $img; do if [ ! -f $fn ]; then echo "$fn doesn't exist."; exit 77; fi; done # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. cat=$topsrc/tests/$prog/cat.txt $execname $img --catalog=$cat --suffix=_wcscat.fits \ --zeroisnotblank --coordcol=4 --coordcol=DEC_CENTER \ --numthreads=1 --mode=wcs --width=3/3600 gnuastro-0.5/tests/crop/imgcat.sh0000755000175000017500000000322013124521441014043 00000000000000# Crop from a catalog using x and y coordinates in Image mode. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=crop img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== # # The number of threads is one so if CFITSIO does is not configured to # enable multithreaded access to files, the tests pass. It is the # users choice to enable this feature. cat=$topsrc/tests/$prog/cat.txt $execname $img --catalog=$cat --suffix=_imgcat.fits --numthreads=1 \ --zeroisnotblank --coordcol=X_CENTER --coordcol=Y_CENTER \ --namecol=NAME --mode=img --width=201 gnuastro-0.5/tests/cosmiccal/0000755000175000017500000000000013217220471013317 500000000000000gnuastro-0.5/tests/cosmiccal/simpletest.sh0000755000175000017500000000213013121462410015756 00000000000000# A simple run of CosmicCalculator to check if it can run. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=cosmiccal execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi # Actual test script # ================== $execname --redshift=2.5 gnuastro-0.5/tests/convolve/0000755000175000017500000000000013217220471013215 500000000000000gnuastro-0.5/tests/convolve/frequency.sh0000755000175000017500000000262013121462410015470 00000000000000# Convolve an image in the frequency domain. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). psf=psf.fits prog=convolve img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi if [ ! -f $psf ]; then echo "$psf does not exist."; exit 77; fi # Actual test script # ================== $execname $img --kernel=$psf --domain=frequency --output=convolve_frequency.fits gnuastro-0.5/tests/convolve/spatial.sh0000755000175000017500000000261213121462410015125 00000000000000# Convolve an image in the spatial domain. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). psf=psf.fits prog=convolve img=mkprofcat1.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi if [ ! -f $psf ]; then echo "$psf does not exist."; exit 77; fi # Actual test script # ================== $execname $img --kernel=$psf --domain=spatial --output=convolve_spatial.fits gnuastro-0.5/tests/convertt/0000755000175000017500000000000013217220471013226 500000000000000gnuastro-0.5/tests/convertt/fitstopdf.sh0000755000175000017500000000265713121462410015514 00000000000000# Convert a FITS image into an PDF file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=convertt img=crop_section.fits execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - Ghostscript was not present on the system. if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi if [ "x$hasghostscript" != "xyes" ]; then echo "Ghostscript 9.10 or above not present."; exit 77; fi # Actual test script # ================== $execname $img --output=pdf --invert gnuastro-0.5/tests/convertt/jpegtofits.sh0000755000175000017500000000262713121462410015665 00000000000000# Convert a FITS image into a one color JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=convertt img=blankch.jpg execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ];then echo "$execname not created.";exit 77;fi if [ ! -f $img ];then echo "$img does not exist."; exit 77;fi if [ "x$haslibjpeg" != "xyes" ];then echo "libjpeg not present."; exit 77;fi # Actual test script # ================== $execname $img --output=fits gnuastro-0.5/tests/convertt/fitstojpegcmyk.sh0000755000175000017500000000264213121462410016546 00000000000000# Convert a FITS image into a JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ];then echo "$execname not created.";exit 77;fi if [ ! -f $img ];then echo "$img does not exist."; exit 77;fi if [ "x$haslibjpeg" != "xyes" ];then echo "libjpeg not present."; exit 77;fi # Actual test script # ================== $execname blank blank blank $img --output=f2jcmyk.jpg gnuastro-0.5/tests/convertt/jpegtotxt.sh0000755000175000017500000000265213121462410015535 00000000000000# Convert a FITS image into a single channel JPEG image to text. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.jpg prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ];then echo "$execname not created.";exit 77;fi if [ ! -f $img ];then echo "$img does not exist."; exit 77;fi if [ "x$haslibjpeg" != "xyes" ];then echo "libjpeg not present."; exit 77;fi # Actual test script # ================== $execname $img --output=jpegtotxt.txt gnuastro-0.5/tests/convertt/blankch.sh0000755000175000017500000000264713121462410015113 00000000000000# Convert a FITS image into a one color JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ];then echo "$execname not created.";exit 77;fi if [ ! -f $img ];then echo "$img does not exist."; exit 77;fi if [ "x$haslibjpeg" != "xyes" ];then echo "libjpeg not present."; exit 77;fi # Actual test script # ================== $execname blank $img blank --output=blankch.jpg gnuastro-0.5/tests/convertt/fitstojpeg.sh0000755000175000017500000000262213121462410015660 00000000000000# Convert a FITS image into a JPEG file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). # # - libjpeg was not present on the system. if [ ! -f $execname ];then echo "$execname not created.";exit 77;fi if [ ! -f $img ];then echo "$img does not exist."; exit 77;fi if [ "x$haslibjpeg" != "xyes" ];then echo "libjpeg not present."; exit 77;fi # Actual test script # ================== $execname $img --invert --output=jpg gnuastro-0.5/tests/convertt/fitstotxt.sh0000755000175000017500000000237713121462410015561 00000000000000# Convert a FITS image into a text file. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=convertt execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img --output=psf.txt gnuastro-0.5/tests/buildprog/0000755000175000017500000000000013217220471013351 500000000000000gnuastro-0.5/tests/buildprog/simpleio.c0000644000175000017500000000342613164537456015302 00000000000000/********************************************************************* A test program to multithreaded building using Gnuastro's helpers. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include "gnuastro/fits.h" int main(int argc, char *argv[]) { gal_data_t *image; char *outname="simpleio.fits"; /* We need two arguments, note that the system also gives the executable name, so argc is one more than the number of arguments. */ if(argc!=3) { fprintf(stderr, "this program only accepts two arguments"); return EXIT_FAILURE; } /* Read the image into memory. */ image=gal_fits_img_read(argv[1], argv[2], -1, 0, 0); /* Let the user know. */ printf("%s (hdu %s) is read into memory.\n", argv[1], argv[2]); /* Save the image in memory into another file. */ gal_fits_img_write(image, outname, NULL, "BuildProgram's Simpleio"); /* Let the user know. */ printf("%s created.\n", outname); /* Clean up and return. */ gal_data_free(image); return EXIT_SUCCESS; } gnuastro-0.5/tests/buildprog/simpleio.sh0000755000175000017500000000404213176441456015465 00000000000000# Make labeled regions on an image with blank pixels. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). img=psf.fits prog=buildprog execname=../bin/$prog/ast$prog source=$topsrc/tests/$prog/simpleio.c # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). # # - The input data was not made (for example the test that created the # data file failed). # # - Gnuastro ships with its own version of Libtool for the building of # the libraries and programs. But here, we want to test the user's # libtool (and how it works with BuildProgram). So if libtool wasn't # found at configure time, we need to skip this test. if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi if [ ! -f $source ]; then echo "$source does not exist."; exit 77; fi if [ "x$hasgnulibtool" != "xyes" ];then echo "GNU libtool not present."; exit 77; fi # Actual test script # ================== # # We want to use the `libgnuastro.la' corresponding to this install, not # the one (that is possibly) installed (hence the use of `--la'). # # Except for `gnuastro/config.h', all headers are installed in # `$topsrc/lib' and `gnuastro/config.h' is in "../lib/" $execname $source $img 1 --la=../lib/libgnuastro.la -I$topsrc/lib -I../lib/ gnuastro-0.5/tests/arithmetic/0000755000175000017500000000000013217220471013513 500000000000000gnuastro-0.5/tests/arithmetic/or.sh0000755000175000017500000000250513124332637014421 00000000000000# Choose two detected regions with the `or' operator # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img 6 eq $img 3 eq or -h2 -h2 --output=or.fits gnuastro-0.5/tests/arithmetic/where.sh0000755000175000017500000000253013121462410015077 00000000000000# Mask non-detected pixels in the image with the `where' operator. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img $img 0 eq nan where -h1 -h2 --output=where.fits gnuastro-0.5/tests/arithmetic/onlynumbers.sh0000755000175000017500000000207613121462410016347 00000000000000# Make an S/N image to test Arithmetic. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi # Actual test script # ================== $execname -1 3.45 x gnuastro-0.5/tests/arithmetic/snimage.sh0000755000175000017500000000253013121462410015410 00000000000000# Make an S/N image to test Arithmetic. # # See the Tests subsection of the manual for a complete explanation # (in the Installing gnuastro section). # # Original author: # Mohammad Akhlaghi # Contributing author(s): # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Preliminaries # ============= # # Set the variables (The executable is in the build tree). Do the # basic checks to see if the executable is made or if the defaults # file exists (basicchecks.sh is in the source tree). prog=arithmetic execname=../bin/$prog/ast$prog img=convolve_spatial_noised_labeled.fits # Skip? # ===== # # If the dependencies of the test don't exist, then skip it. There are two # types of dependencies: # # - The executable was not made (for example due to a configure option), # # - The input data was not made (for example the test that created the # data file failed). if [ ! -f $execname ]; then echo "$execname not created."; exit 77; fi if [ ! -f $img ]; then echo "$img does not exist."; exit 77; fi # Actual test script # ================== $execname $img $img - $img / --hdu=1 --hdu=4 --hdu=5 \ --output=snimage.fits gnuastro-0.5/doc/0000755000175000017500000000000013217220467010772 500000000000000gnuastro-0.5/doc/gnuastro.info-50000644000175000017500000066321513217220437013605 00000000000000This is gnuastro.info, produced by makeinfo version 6.5 from gnuastro.texi. This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro’s library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Building and debugging, Next: Test scripts, Prev: Documentation, Up: Developing 11.6 Building and debugging =========================== To build the various programs and libraries in Gnuastro, the GNU build system is used which defines the steps in *note Quick start::. It consists of GNU Autoconf, GNU Automake and GNU Libtool which are collectively known as GNU Autotools. They provide a very portable system to check the hosts environment and compile Gnuastro based on that. They also make installing everything in their standard places very easy for the programmer. Most of the small caps files that you see in the top source directory of the tarball are created by these three tools (see *note Version controlled source::). To facilitate the building and testing of your work during development, Gnuastro comes with two useful scripts: ‘tmpfs-config-make’ This is more fully described in *note Configure and build in RAM::. During development, you will usually run this command only once (at the start of your work). ‘tests/during-dev.sh’ This script is designed to be run each time you make a change and want to test your work (with some possible input and output). The script itself is heavily commented and thoroughly describes the best way to use it, so we won’t repeat it here. As a short summary: you specify the build directory, an output directory (for the built program to be run in, and also contains the inputs), the program’s short name and the arguments and options that it should be run with. This script will then build Gnuastro, go to the output directory and run the built executable from there. One option for the output directory might be your desktop, so you can easily see the output files and delete them when you are finished. The main purpose of these scripts is to keep your source directory clean and facilitate your development. By default all the programs are compiled with optimization flags for increased speed. A side effect of optimization is that valuable debugging information is lost. All the libraries are also linked as shared libraries by default. Shared libraries further complicate the debugging process and significantly slow down the compilation (the ‘make’ command). So during development it is recommended to configure Gnuastro as follows: $ ./configure --disable-shared CFLAGS="-g -O0" In ‘tmpfs-config-make’ you can ask for this behavior by setting ‘debug_noshared’ to ‘1’. In order to understand the building process, you can go through the Autoconf, Automake and Libtool manuals, like all GNU manuals they provide both a great tutorial and technical documentation. The “A small Hello World†section in Automake’s manual (in chapter 2) can be a good starting guide after you have read the separate introductions.  File: gnuastro.info, Node: Test scripts, Next: Developer's checklist, Prev: Building and debugging, Up: Developing 11.7 Test scripts ================= As explained in *note Tests::, for every program some simple tests are written to check the various independent features of the program. All the tests are placed in the ‘tests/’ directory. The ‘tests/prepconf.sh’ script is the first ‘test’ that will be run. It will copy all the configuration files from the various directories to a ‘tests/.gnuastro’ directory (which it will make) so the various tests can set the default values. This script will also make sure the programs don’t go searching for user and system wide configuration files to avoid the mixing of values with different Gnuastro version on the system. For each program, the tests are placed inside directories with the program name. Each test is written as a shell script. The last line of this script is the test which runs the program with certain parameters. The return value of this script determines the fate of the test, see the “Support for test suites†chapter of the Automake manual for a very nice and complete explanation. In every script, two variables are defined at first: ‘prog’ and ‘execname’. The first specifies the program name and the second the location of the executable. The most important thing to have in mind about all the test scripts is that they are run from inside the ‘tests/’ directory in the “build treeâ€. Which can be different from the directory they are stored in (known as the “source treeâ€)(1). This distinction is made by GNU Autoconf and Automake (which configure, build and install Gnuastro) so that you can install the program even if you don’t have write access to the directory keeping the source files. See the “Parallel build trees (a.k.a VPATH builds)†in the Automake manual for a nice explanation. Because of this, any necessary inputs that are distributed in the tarball(2), for example the catalogs necessary for checks in MakeProfiles and Crop, must be identified with the ‘$topsrc’ prefix instead of ‘../’ (for the top source directory that is unpacked). This ‘$topsrc’ variable points to the source tree where the script can find the source data (it is defined in ‘tests/Makefile.am’). The executables and other test products were built in the build tree (where they are being run), so they don’t need to be prefixed with that variable. This is also true for images or files that were produced by other tests. ---------- Footnotes ---------- (1) The ‘tmpfs-config-make’ script also uses this feature to keep the source and build directories separate (see *note Configure and build in RAM::). (2) In many cases, the inputs of a test are outputs of previous tests, this doesn’t apply to this class of inputs. Because all outputs of previous tests are in the “build treeâ€.  File: gnuastro.info, Node: Developer's checklist, Next: Gnuastro project webpage, Prev: Test scripts, Up: Developing 11.8 Developer’s checklist ========================== This is a checklist of things to do after applying your changes/additions in Gnuastro: 1. If the change is non-trivial, write test(s) in the ‘tests/progname/’ directory to test the change(s)/addition(s) you have made. Then add their file names to ‘tests/Makefile.am’. 2. Run ‘$ make check’ to make sure everything is working correctly. 3. Make sure the documentation (this book) is completely up to date with your changes, see *note Documentation::. 4. Commit the change to your issue branch (see *note Production workflow:: and *note Forking tutorial::). Afterwards, run Autoreconf to generate the appropriate version number: $ autoreconf -f 5. Finally, to make sure everything will be built, installed and checked correctly run the following command (after re-configuring, and re-building). To greatly speed up the process, use multiple threads (8 in the example below, change it appropriately) $ make distcheck -j8 This command will create a distribution file (ending with ‘.tar.gz’) and try to compile it in the most general cases, then it will run the tests on what it has built in its own mini-environment. If ‘$ make distcheck’ finishes successfully, then you are safe to send your changes to us to implement or for your own purposes. See *note Production workflow:: and *note Forking tutorial::.  File: gnuastro.info, Node: Gnuastro project webpage, Next: Developing mailing lists, Prev: Developer's checklist, Up: Developing 11.9 Gnuastro project webpage ============================= Gnuastro’s central management hub (https://savannah.gnu.org/projects/gnuastro/)(1) is located on GNU Savannah (https://savannah.gnu.org/)(2). Savannah is the central software development management system for many GNU projects. Through this central hub, you can view the list of activities that the developers are engaged in, their activity on the version controlled source, and other things. Each defined activity in the development cycle is known as an ‘issue’ (or ‘item’). An issue can be a bug (see *note Report a bug::), or a suggested feature (see *note Suggest new feature::) or an enhancement or generally any _one_ job that is to be done. In Savannah, issues are classified into three categories or ‘tracker’s: Support This tracker is a way that (possibly anonymous) users can get in touch with the Gnuastro developers. It is a complement to the bug-gnuastro mailing list (see *note Report a bug::). Anyone can post an issue to this tracker. The developers will not submit an issue to this list. They will only reassign the issues in this list to the other two trackers if they are valid(3). Ideally (when the developers have time to put on Gnuastro, please don’t forget that Gnuastro is a volunteer effort), there should be no open items in this tracker. Bugs This tracker contains all the known bugs in Gnuastro (problems with the existing tools). Tasks The items in this tracker contain the future plans (or new features/capabilities) that are to be added to Gnuastro. All the trackers can be browsed by a (possibly anonymous) visitor, but to edit and comment on the Bugs and Tasks trackers, you have to be a registered on Savannah. When posting an issue to a tracker, it is very important to choose the ‘Category’ and ‘Item Group’ options accurately. The first contains a list of all Gnuastro’s programs along with ‘Installation’, ‘New program’ and ‘Webpage’. The “Item Group†contains the nature of the issue, for example if it is a ‘Crash’ in the software (a bug), or a problem in the documentation (also a bug) or a feature request or an enhancement. The set of horizontal links on the top of the page (Starting with ‘Main’ and ‘Homepage’ and finishing with ‘News’) are the easiest way to access these trackers (and other major aspects of the project) from any part of the project webpage. Hovering your mouse over them will open a drop down menu that will link you to the different things you can do on each tracker (for example, ‘Submit new’ or ‘Browse’). When you browse each tracker, you can use the “Display Criteria†link above the list to limit the displayed issues to what you are interested in. The ‘Category’ and ‘Group Item’ (explained above) are a good starting point. Any new issue that is submitted to any of the trackers, or any comments that are posted for an issue, is directly forwarded to the gnuastro-devel mailing list (, see *note Developing mailing lists:: for more). This will allow anyone interested to be up to date on the over-all development activity in Gnuastro and will also provide an alternative (to Savannah) archiving for the development discussions. Therefore, it is not recommended to directly post an email to this mailing list, but do all the activities (for example add new issues, or comment on existing ones) on Savannah. *Do I need to be a member in Savannah to contribute to Gnuastro?* No. The full version controlled history of Gnuastro is available for anonymous download or cloning. See *note Production workflow:: for a description of Gnuastro’s Integration-Manager Workflow. In short, you can either send in patches, or make your own fork. If you choose the latter, you can push your changes to your own fork and inform us. We will then pull your changes and merge them into the main project. Please see *note Forking tutorial:: for a tutorial. ---------- Footnotes ---------- (1) (2) (3) Some of the issues registered here might be due to a mistake on the user’s side, not an actual bug in the program.  File: gnuastro.info, Node: Developing mailing lists, Next: Contributing to Gnuastro, Prev: Gnuastro project webpage, Up: Developing 11.10 Developing mailing lists ============================== To keep the developers and interested users up to date with the activity and discussions within Gnuastro, there are two mailing lists which you can subscribe to: ‘gnuastro-devel@gnu.org’ (at ) All the posts made in the support, bugs and tasks discussions of *note Gnuastro project webpage:: are also sent to this mailing address and archived. By subscribing to this list you can stay up to date with the discussions that are going on between the developers before, during and (possibly) after working on an issue. All discussions are either in the context of bugs or tasks which are done on Savannah and circulated to all interested people through this mailing list. Therefore it is not recommended to post anything directly to this mailing list. Any mail that is sent to it from Savannah to this list has a link under the title “Reply to this item at:â€. That link will take you directly to the issue discussion page, where you can read the discussion history or join it. While you are posting comments on the Savannah issues, be sure to update the meta-data. For example if the task/bug is not assigned to anyone and you would like to take it, change the “Assigned to†box, or if you want to report that it has been applied, change the status and so on. All these changes will also be circulated with the email very clearly. ‘gnuastro-commits@gnu.org’ (at ) This mailing list is defined to circulate all commits that are done in Gnuastro’s version controlled source, see *note Version controlled source::. If you have any ideas, or suggestions on the commits, please use the bug and task trackers on Savannah to followup the discussion, do not post to this list. All the commits that are made for an already defined issue or task will state the respective ID so you can find it easily.  File: gnuastro.info, Node: Contributing to Gnuastro, Prev: Developing mailing lists, Up: Developing 11.11 Contributing to Gnuastro ============================== You have this great idea or have found a good fix to a problem which you would like to implement in Gnuastro. You have also become familiar with the general design of Gnuastro in the previous sections of this chapter (see *note Developing::) and want to start working on and sharing your new addition/change with the whole community as part of the official release. This is great and your contribution is most welcome. This section and the next (see *note Developer's checklist::) are written in the hope of making it as easy as possible for you to share your great idea with the community. In this section we discuss the final steps you have to take: legal and technical. From the legal perspective, the copyright of any work you do on Gnuastro has to be assigned to the Free Software Foundation (FSF) and the GNU operating system, or you have to sign a disclaimer. We do this to ensure that Gnuastro can remain free in the future, see *note Copyright assignment::. From the technical point of view, in this section we also discuss commit guidelines (*note Commit guidelines::) and the general version control workflow of Gnuastro in *note Production workflow::, along with a tutorial in *note Forking tutorial::. Recall that before starting the work on your idea, be sure to checkout the bugs and tasks trackers in *note Gnuastro project webpage:: and announce your work there so you don’t end up spending time on something others have already worked on, and also to attract similarly interested developers to help you. * Menu: * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git.  File: gnuastro.info, Node: Copyright assignment, Next: Commit guidelines, Prev: Contributing to Gnuastro, Up: Contributing to Gnuastro 11.11.1 Copyright assignment ---------------------------- Gnuastro’s copyright is owned by the FSF. Professor Eben Moglen, of the Columbia University Law School has given a nice summary of the reasons for this at . Below we are copying it verbatim for self consistency (in case you are offline or reading in print). Under US copyright law, which is the law under which most free software programs have historically been first published, there are very substantial procedural advantages to registration of copyright. And despite the broad right of distribution conveyed by the GPL, enforcement of copyright is generally not possible for distributors: only the copyright holder or someone having assignment of the copyright can enforce the license. If there are multiple authors of a copyrighted work, successful enforcement depends on having the cooperation of all authors. In order to make sure that all of our copyrights can meet the record keeping and other requirements of registration, and in order to be able to enforce the GPL most effectively, FSF requires that each author of code incorporated in FSF projects provide a copyright assignment, and, where appropriate, a disclaimer of any work-for-hire ownership claims by the programmer’s employer. That way we can be sure that all the code in FSF projects is free code, whose freedom we can most effectively protect, and therefore on which other developers can completely rely. Please get in touch with the Gnuastro maintainer (currently Mohammad Akhlaghi, akhlaghi -at- gnu -dot- org) to follow the procedures. It is possible to do this for each change (good for for a single contribution), and also more generally for all the changes/additions you do in the future within Gnuastro. So if you have already assigned the copyright of your work on another GNU software to the FSF, it should be done again for Gnuastro. The FSF has staff working on these legal issues and the maintainer will get you in touch with them to do the paperwork. The maintainer will just be informed in the end so your contributions can be merged within the Gnuastro source code. Gnuastro will gratefully acknowledge (see *note Acknowledgments::) all the people who have assigned their copyright to the FSF and have thus helped to guarantee the freedom and reliability of Gnuastro. The Free Software Foundation will also acknowledge your copyright contributions in the Free Software Supporter: which will circulate to a very large community (104,444 people in April 2016). See the archives for some examples and subscribe to receive interesting updates. The very active code contributors (or developers) will also be recognized as project members on the Gnuastro project webpage (see *note Gnuastro project webpage::) and can be given a ‘gnu.org’ email address. So your very valuable contribution and copyright assignment will not be forgotten and is highly appreciated by a very large community. If you are reluctant to sign an assignment, a disclaimer is also acceptable. *Do I need a disclaimer from my university or employer?* It depends on the contract with your university or employer. From the FSF’s ‘/gd/gnuorg/conditions.text’: “If you are employed to do programming, or have made an agreement with your employer that says it owns programs you write, we need a signed piece of paper from your employer disclaiming rights to†Gnuastro. The FSF’s copyright clerk will kindly help you decide, please consult the following email address: “assign -at- gnu -dot- orgâ€.  File: gnuastro.info, Node: Commit guidelines, Next: Production workflow, Prev: Copyright assignment, Up: Contributing to Gnuastro 11.11.2 Commit guidelines ------------------------- To be able to cleanly integrate your work with the other developers, *never commit on the ‘master’ branch* (see *note Production workflow:: for a complete discussion and *note Forking tutorial:: for a cookbook example). In short, leave ‘master’ only for changes you fetch, or pull from the official repository (see *note Synchronizing::). In the Gnuastro commit messages, we strive to follow these standards. Note that in the early phases of Gnuastro’s development, we are experimenting and so if you notice earlier commits don’t satisfy some of the guidelines below, it is because they predate that guideline. Commit title The commits have to start with one short descriptive title. The title is separated from the body with one blank line. Run ‘git log’ to see some of the most recent commit messages as an example. In general, the title should satisfy the following conditions: • It is best for the title to be short, about 60 (or even 50) characters. Most emulated command-line terminals are about 80 characters wide. However, we should also allow for the commit hashes which are printed in ‘git log --oneline’, and also branch names or the graph structure outputs of ‘git log’ which are also commonly used. • The title should not finish with any full-stops or periods (‘<.>’). Commit body The body of the commit message is separated from the title by one empty line. Recall that anyone who has subscribed to ‘gnuastro-commits’ mailing list will get the commit in their email after it has been pushed to ‘master’. People will also read them when they synchronize with the main Gnuastro repository (see *note Synchronizing::). Finally, the commit messages will later be used to update the ‘NEWS’ file on each release. Therefore the commit message body plays a very important role in the development of Gnuastro, so please adhere to the following guidelines. • The body should be very descriptive. Start the commit message body by explaining what changes your commit makes from a user’s perspective (added, changed, or removed options, or arguments to programs or libraries, or modified algorithms, or new installation step, or etc). • Try to explain the committed contents as best as you can. Recall that the readers of your commit message do not necessarily have your current background. After some time you will also forget the context, so this request is not just for others(1). Therefore be very descriptive and explain as much as possible: what the bug/task was, justify the way you fixed it and discuss other possible solutions that you might not have included. For the last item, it is best to discuss them thoroughly as comments in the appropriate section of the code, but only give a short summary in the commit message. Note that all added and removed source code lines will also be circulated in the ‘gnuastro-commits’ mailing list. • Like all other Gnuastro’s text files, the lines in the commit body should not be longer than 75 characters, see *note Coding conventions::. This is to ensure that on standard terminal emulators (with 80 character width), the ‘git log’ output can be cleanly displayed (note that the commit message is indented in the output of ‘git log’). If you use Emacs, Gnuastro’s ‘.dir-locals.el’ file will ensure that your commits satisfy this condition (using ). • When the commit is related to a task or a bug, please include the respective ID (in the format of ‘bug/task #ID’, note the space) in the commit message (from *note Gnuastro project webpage::) for interested people to be able to followup the discussion that took place there. If the commit fixes a bug or finishes a task, the recommended way is to add a line after the body with ‘‘This fixes bug #ID.’’, or ‘‘This finishes task #ID.’’. Don’t assume that the reader has internet access to check the bug’s full description when reading the commit message, so give a short introduction too. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Production workflow, Next: Forking tutorial, Prev: Commit guidelines, Up: Contributing to Gnuastro 11.11.3 Production workflow --------------------------- Fortunately ‘Pro Git’ has done a wonderful job in explaining the different workflows in Chapter 5(1) and in particular the “Integration-Manager Workflow†explained there. The implementation of this workflow is nicely explained in Section 5.2(2) under “Forked-Public-Projectâ€. We have also prepared a short tutorial in *note Forking tutorial::. Anything on the master branch should always be tested and ready to be built and used. As described in ‘Pro Git’, there are two methods for you to contribute to Gnuastro in the Integration-Manager Workflow: 1. You can send commit patches by email as fully explained in ‘Pro Git’. This is good for your first few contributions. Just note that raw patches (containing only the diff) do not have any meta-data (author name, date and etc). Therefore they will not allow us to fully acknowledge your contributions as an author in Gnuastro: in the ‘AUTHORS’ file and at the start of the PDF book. These author lists are created automatically from the version controlled source. To receive full acknowledgment when submitting a patch, is thus advised to use Git’s ‘format-patch’ tool. See Pro Git’s Public project over email (https://git-scm.com/book/en/v2/Distributed-Git-Contributing-to-a-Project#Public-Project-over-Email) section for a nice explanation. If you would like to get more heavily involved in Gnuastro’s development, then you can try the next solution. 2. You can have your own forked copy of Gnuastro on any hosting site you like (GitHub, GitLab, BitBucket, or etc) and inform us when your changes are ready so we merge them in Gnuastro. This is more suited for people who commonly contribute to the code (see *note Forking tutorial::). In both cases, your commits (with your name and information) will be preserved and your contributions will thus be fully recorded in the history of Gnuastro and in the ‘AUTHORS’ file and this book (second page in the PDF format) once they have been incorporated into the official repository. Needless to say that in such cases, be sure to follow the bug or task trackers (or subscribe to the ‘gnuastro-devel’ mailing list) and contact us before hand so you don’t do something that someone else is already working on. In that case, you can get in touch with them and help the job go on faster, see *note Gnuastro project webpage::. This workflow is currently mostly borrowed from the general recommendations of Git(3) and GitHub. But since Gnuastro is currently under heavy development, these might change and evolve to better suit our needs. ---------- Footnotes ---------- (1) (2) (3)  File: gnuastro.info, Node: Forking tutorial, Prev: Production workflow, Up: Contributing to Gnuastro 11.11.4 Forking tutorial ------------------------ This is a tutorial on the second suggested method (commonly known as forking) that you can submit your modifications in Gnuastro (see *note Production workflow::). To start, please create an empty repository on your hosting service webpage (we recommend GitLab(1)). If this is your first hosted repository on the webpage, you also have to upload your public SSH key(2) for the ‘git push’ command below to work. Here we’ll assume you use the name ‘janedoe’ to refer to yourself everywhere and that you choose ‘gnuastro-janedoe’ as the name of your Gnuastro fork. Any online hosting service will give you an address (similar to the ‘‘git@gitlab.com:...’’ below) of the empty repository you have created using their webpage, use that address in the third line below. $ git clone git://git.sv.gnu.org/gnuastro.git $ cd gnuastro $ git remote add janedoe git@gitlab.com:janedoe/gnuastro-janedoe.git $ git push janedoe master The full Gnuastro history is now pushed onto your hosting service and the ‘janedoe’ remote is now also following your ‘master’ branch. If you run ‘git remote show REMOTENAME’ for the ‘origin’ and ‘janedoe’ remotes, you will see their difference: the first has pull access and the second doesn’t. This nicely summarizes the main idea behind this workflow: you push to your remote repository, we pull from it and merge it into ‘master’, then you finalize it by pulling from the main repository. To test (compile) your changes during your work, you will need to bootstrap the version controlled source, see *note Bootstrapping:: for a full description. The cloning process above is only necessary for your first time setup, you don’t need to repeat it. However, please repeat the steps below for each independent issue you intend to work on. Let’s assume you have found a bug in ‘lib/statistics.c’’s median calculating function. Before actually doing anything, please announce it (see *note Report a bug::) so everyone knows you are working on it or to find out others aren’t already working on it. With the commands below, you make a branch, checkout to it, correct the bug, check if it is indeed fixed, add it to the staging area, commit it to the new branch and push it to your hosting service. But before all of them, make sure that you are on the ‘master’ branch and that your ‘master’ branch is up to date with the main Gnuastro repository with the first two commands. $ git checkout master $ git pull $ git checkout -b bug-median-stats # Choose a descriptive name $ emacs lib/statistics.c $ # do your checks here $ git add lib/statistics.c $ git commit $ git push janedoe bug-median-stats Your new branch is now on your hosted repository. Through the respective tacker on Savannah (see *note Gnuastro project webpage::) you can then let the other developers know that your ‘bug-median-stats’ branch is ready. They will pull your work, test it themselves and if it is ready to be merged into the main Gnuastro history, they will merge it into the ‘master’ branch. After that is done, you can simply checkout your local ‘master’ branch and pull all the changes from the main repository. After the pull you can run ‘‘git log’’ as shown below, to see how ‘bug-median-stats’ is merged with master. To finalize, you can push all the changes to your hosted repository and delete the branch: $ git checkout master $ git pull $ git log --oneline --graph --decorate --all $ git push janedoe master $ git branch -d bug-median-stats # delete local branch $ git push janedoe --delete bug-median-stats # delete remote branch Just as a reminder, always keep your work on each issue in a separate local and remote branch so work can progress on them independently. After you make your announcement, other people might contribute to the branch before merging it in to ‘master’, so this is very important. As a final reminder: before starting each issue branch from ‘master’, be sure to run ‘git pull’ in ‘master’ as shown above. This will enable you to start your branch (work) from the most recent commit and thus simplify the final merging of your work. ---------- Footnotes ---------- (1) See for an evaluation of the major existing repositories. Gnuastro uses GNU Savannah (which also has the highest ranking in the evaluation), but for starters, GitLab may be easier. (2) For example see this explanation provided by GitLab: .  File: gnuastro.info, Node: Gnuastro programs list, Next: Other useful software, Prev: Developing, Up: Top Appendix A Gnuastro programs list ********************************* GNU Astronomy Utilities 0.5, contains the following programs. They are sorted in alphabetical order and a short description is provided for each program. The description starts with the executable names in ‘thisfont’ followed by a pointer to the respective section in parenthesis. Throughout this book, they are ordered based on their context, please see the top-level contents for contextual ordering (based on what they do). Arithmetic (‘astarithmetic’, see *note Arithmetic::) For arithmetic operations on multiple (theoretically unlimited) number of datasets (images). It has a large and growing set of arithmetic, mathematical, and even statistical operators (for example ‘+’, ‘-’, ‘*’, ‘/’, ‘sqrt’, ‘log’, ‘min’, ‘average’, ‘median’). BuildProgram (‘astbuildprog’, see *note BuildProgram::) Compile, link and run programs that depend on the Gnuastro library (see *note Gnuastro library::). This program will automatically link with the libraries that Gnuastro depends on, so there is no need to explicitly mention them every time you are compiling a Gnuastro library dependent program. ConvertType (‘astconvertt’, see *note ConvertType::) Convert astronomical data files (FITS or IMH) to and from several other standard image and data formats, for example TXT, JPEG, EPS or PDF. Convolve (‘astconvolve’, see *note Convolve::) Convolve (blur or smooth) data with a given kernel in spatial and frequency domain on multiple threads. Convolve can also do de-convolution to find the appropriate kernel to PSF-match two images. CosmicCalculator (‘astcosmiccal’, see *note CosmicCalculator::) Do cosmological calculations, for example the luminosity distance, distance modulus, comoving volume and many more. Crop (‘astcrop’, see *note Crop::) Crop region(s) from an image and stitch several images if necessary. Inputs can be in pixel coordinates or world coordinates. Fits (‘astfits’, see *note Fits::) View and manipulate FITS file extensions and header keywords. Statistics (‘aststatistics’, see *note Statistics::) Get pixel statistics and save histogram and cumulative frequency plots. MakeCatalog (‘astmkcatalog’, see *note MakeCatalog::) Make catalog of labeled image (output of NoiseChisel). The catalogs are highly customizable and adding new calculations/columns is very straightforward. MakeNoise (‘astmknoise’, see *note MakeNoise::) Make (add) noise to an image, with a large set of random number generators and any seed. MakeProfiles (‘astmkprof’, see *note MakeProfiles::) Make mock 2D profiles in an image. The central regions of radial profiles are made with a configurable 2D Monte Carlo integration. It can also build the profiles on an over-sampled image. Match (‘astmatch’, see *note Match::) Given two input catalogs, find the rows that match with each other within a given aperture (may be an ellipse). NoiseChisel (‘astnoisechisel’, see *note NoiseChisel::) Detect and segment signal in noise. It uses a technique to detect very faint and diffuse, irregularly shaped signal in noise (galaxies in the sky), using thresholds that are below the Sky value, see arXiv:1505.01664 (http://arxiv.org/abs/1505.01664). Table (‘asttable’, *note Table::) Convert FITS binary and ASCII tables into other such tables, print them on the command-line, save them in a plain text file, or get the FITS table information. Warp (‘astwarp’, see *note Warp::) Warp image to new pixel grid. Any projective transformation or Homography can be applied to the input images.  File: gnuastro.info, Node: Other useful software, Next: GNU Free Doc. License, Prev: Gnuastro programs list, Up: Top Appendix B Other useful software ******************************** In this appendix the installation of programs and libraries that are not direct Gnuastro dependencies are discussed. However they can be useful for working with Gnuastro. * Menu: * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C  File: gnuastro.info, Node: SAO ds9, Next: PGPLOT, Prev: Other useful software, Up: Other useful software B.1 SAO ds9 =========== SAO ds9(1) is not a requirement of Gnuastro, it is a FITS image viewer. So to check your inputs and outputs, it is one of the best options. Like the other packages, it might already be available in your distribution’s repositories. It is already pre-compiled in the download section of its webpage. Once you download it you can unpack and install (move it to a system recognized directory) with the following commands (‘x.x.x’ is the version number): $ tar xf ds9.linux64.x.x.x.tar.gz $ sudo mv ds9 /usr/local/bin Once you run it, there might be a complaint about the Xss library, which you can find in your distribution package management system. You might also get an ‘XPA’ related error. In this case, you have to add the following line to your ‘~/.bashrc’ and ‘~/.profile’ file (you will have to log out and back in again for the latter): export XPA_METHOD=local * Menu: * Viewing multiextension FITS images:: Configure SAO ds9 for multiextension images. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Viewing multiextension FITS images, Prev: SAO ds9, Up: SAO ds9 B.1.1 Viewing multiextension FITS images ---------------------------------------- The FITS definition allows for multiple extensions inside a FITS file, each extension can have a completely independent data set inside of it. If you ordinarily open a multi-extension FITS file with SAO ds9, for example by double clicking on the file or running ‘$ds9 foo.fits’, SAO ds9 will only show you the first extension. To be able to switch between the extensions you have to follow these menus in the SAO ds9 window: File→Open Other→Open Multi Ext Cube and then choose the Multi extension FITS file in your computer’s file structure. The method above is a little tedious to do every time you want view a multi-extension FITS file. Fortunately SAO ds9 also provides options that you can use to specify a particular behavior. One of those options is ‘-mecube’ which opens a FITS image as a multi-extension data cube. So on the command-line, if you run ‘$ds9 -mecube foo.fits’ a small window will also be opened, which allows you to switch between the image extensions that ‘foo.fits’ might have. If ‘foo.fits’ only consists of one extension, then SAO ds9 will open as usual. Just to avoid confusion, note that SAO ds9 does not follow the GNU style of separating long and short options as explained in *note Arguments and options::. In the GNU style, this ‘long’ option should have been called like ‘--mecube’, but SAO ds9 does follow those conventions and has its own. It is really convenient if you set ds9 to always run with the ‘-mecube’ option on your graphical display. On GNOME 3 (the most popular graphic user interface for GNU/Linux systems) you can do this by taking the following steps: • Open your favorite text editor and put the following text in a file that ends with ‘.desktop’, for example ‘saods9.desktop’. The file is very descriptive. [Desktop Entry] Type=Application Version=1.0 Name=SAO ds9 Comment=View FITS images Exec=ds9 -mecube %f Terminal=false Categories=Graphic;FITS; • Copy this file into your local (user) applications directory: $ cp saods9.desktop ~/.local/share/applications/ In case you don’t have the directory, you can make it yourself: $ mkdir -p ~/.local/share/applications/ • The steps above will add SAO ds9 as one of your applications. To make it default for every time you click on a FITS file. Right click on a FITS file and select “Open Withâ€, then go into “Other Application...†and choose “SAO ds9â€. In case you are using GNOME 2 you can take the following steps: right click on a FITS file and choose Properties→Open With→Add button. A list of applications will show up, ds9 might already be present in the list, but don’t choose it because it will run with no options. Below the list is an option “Use a custom commandâ€. Click on it and write the following command: ‘ds9 -mecube’ in the box and click “Addâ€. Then finally choose the command you just added as the default and click the “Close†button.  File: gnuastro.info, Node: PGPLOT, Prev: SAO ds9, Up: Other useful software B.2 PGPLOT ========== PGPLOT is a package for making plots in C. It is not directly needed by Gnuastro, but can be used by WCSLIB, see *note WCSLIB::. As explained in *note WCSLIB::, you can install WCSLIB without it too. It is very old (the most recent version was released early 2001!), but remains one of the main packages for plotting directly in C. WCSLIB uses this package to make plots if you want it to make plots. If you are interested you can also use it for your own purposes. If you want your plotting codes in between your C program, PGPLOT is currently one of your best options. The recommended alternative to this method is to get the raw data for the plots in text files and input them into any of the various more modern and capable plotting tools separately, for example the Matplotlib library in Python or PGFplots in LaTeX. This will also significantly help code readability. Let’s get back to PGPLOT for the sake of WCSLIB. Installing it is a little tricky (mainly because it is so old!). You can download the most recent version from the FTP link in its webpage(1). You can unpack it with the ‘tar xf’ command. Let’s assume the directory you have unpacked it to is ‘PGPLOT’, most probably it is: ‘/home/username/Downloads/pgplot/’. open the ‘drivers.list’ file: $ gedit drivers.list Remove the ‘!’ for the following lines and save the file in the end: PSDRIV 1 /PS PSDRIV 2 /VPS PSDRIV 3 /CPS PSDRIV 4 /VCPS XWDRIV 1 /XWINDOW XWDRIV 2 /XSERVE Don’t choose GIF or VGIF, there is a problem in their codes. Open the ‘PGPLOT/sys_linux/g77_gcc.conf’ file: $ gedit PGPLOT/sys_linux/g77_gcc.conf change the line saying: ‘FCOMPL="g77"’ to ‘FCOMPL="gfortran"’, and save it. This is a very important step during the compilation of the code if you are in GNU/Linux. You now have to create a folder in ‘/usr/local’, don’t forget to replace ‘PGPLOT’ with your unpacked address: $ su # mkdir /usr/local/pgplot # cd /usr/local/pgplot # cp PGPLOT/drivers.list ./ To make the Makefile, type the following command: # PGPLOT/makemake PGPLOT linux g77_gcc It should finish by saying: ‘Determining object file dependencies’. You have done the hard part! The rest is easy: run these three commands in order: # make # make clean # make cpg Finally you have to place the position of this directory you just made into the ‘LD_LIBRARY_PATH’ environment variable and define the environment variable ‘PGPLOT_DIR’. To do that, you have to edit your ‘.bashrc’ file: $ cd ~ $ gedit .bashrc Copy these lines into the text editor and save it: PGPLOT_DIR="/usr/local/pgplot/"; export PGPLOT_DIR LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/pgplot/ export LD_LIBRARY_PATH You need to log out and log back in again so these definitions take effect. After you logged back in, you want to see the result of all this labor, right? Tim Pearson has done that for you, create a temporary folder in your home directory and copy all the demonstration files in it: $ cd ~ $ mkdir temp $ cd temp $ cp /usr/local/pgplot/pgdemo* ./ $ ls You will see a lot of pgdemoXX files, where XX is a number. In order to execute them type the following command and drink your coffee while looking at all the beautiful plots! You are now ready to create your own. $ ./pgdemoXX ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: GNU Free Doc. License, Next: Index, Prev: Other useful software, Up: Top Appendix C GNU Free Doc. License ******************************** Version 1.3, 3 November 2008 Copyright © 2000, 2001, 2002, 2007, 2008 Free Software Foundation, Inc. Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. 0. PREAMBLE The purpose of this License is to make a manual, textbook, or other functional and useful document “free†in the sense of freedom: to assure everyone the effective freedom to copy and redistribute it, with or without modifying it, either commercially or noncommercially. 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If you have Invariant Sections, Front-Cover Texts and Back-Cover Texts, replace the “with...Texts.†line with this: with the Invariant Sections being LIST THEIR TITLES, with the Front-Cover Texts being LIST, and with the Back-Cover Texts being LIST. If you have Invariant Sections without Cover Texts, or some other combination of the three, merge those two alternatives to suit the situation. If your document contains nontrivial examples of program code, we recommend releasing these examples in parallel under your choice of free software license, such as the GNU General Public License, to permit their use in free software.  File: gnuastro.info, Node: Index, Prev: GNU Free Doc. License, Up: Top Index: Macros, structures and functions *************************************** All Gnuastro library’s exported macros start with ‘GAL_’, and its exported structures and functions start with ‘gal_’. This abbreviation stands for _G_NU _A_stronomy _L_ibrary. The next element in the name is the name of the header which declares or defines them, so to use the ‘gal_array_fset_const’ function, you have to ‘#include ’. See *note Gnuastro library:: for more. The ‘pthread_barrier’ constructs are our implementation and are only available on systems that don’t have them, see *note Implementation of pthread_barrier::. [index] * Menu: * gal_arithmetic: Arithmetic on datasets. (line 222) * GAL_ARITHMETIC_FLAGS_ALL: Arithmetic on datasets. (line 39) * GAL_ARITHMETIC_FREE: Arithmetic on datasets. (line 37) * GAL_ARITHMETIC_INPLACE: Arithmetic on datasets. (line 36) * GAL_ARITHMETIC_NUMOK: Arithmetic on datasets. (line 38) * GAL_ARITHMETIC_OP_ABS: Arithmetic on datasets. (line 152) * GAL_ARITHMETIC_OP_AND: Arithmetic on datasets. (line 74) * GAL_ARITHMETIC_OP_BITAND: Arithmetic on datasets. (line 176) * GAL_ARITHMETIC_OP_BITLSH: Arithmetic on datasets. (line 179) * GAL_ARITHMETIC_OP_BITNOT: Arithmetic on datasets. (line 196) * GAL_ARITHMETIC_OP_BITOR: Arithmetic on datasets. (line 177) * GAL_ARITHMETIC_OP_BITRSH: Arithmetic on datasets. (line 180) * GAL_ARITHMETIC_OP_BITXOR: Arithmetic on datasets. (line 178) * GAL_ARITHMETIC_OP_DIVIDE: Arithmetic on datasets. (line 67) * GAL_ARITHMETIC_OP_EQ: Arithmetic on datasets. (line 72) * GAL_ARITHMETIC_OP_GE: Arithmetic on datasets. (line 71) * GAL_ARITHMETIC_OP_GT: Arithmetic on datasets. (line 70) * GAL_ARITHMETIC_OP_ISBLANK: Arithmetic on datasets. (line 96) * GAL_ARITHMETIC_OP_LE: Arithmetic on datasets. (line 69) * GAL_ARITHMETIC_OP_LOG: Arithmetic on datasets. (line 126) * GAL_ARITHMETIC_OP_LOG10: Arithmetic on datasets. (line 127) * GAL_ARITHMETIC_OP_LT: Arithmetic on datasets. (line 68) * GAL_ARITHMETIC_OP_MAX: Arithmetic on datasets. (line 156) * GAL_ARITHMETIC_OP_MAXVAL: Arithmetic on datasets. (line 139) * GAL_ARITHMETIC_OP_MEAN: Arithmetic on datasets. (line 159) * GAL_ARITHMETIC_OP_MEANVAL: Arithmetic on datasets. (line 142) * GAL_ARITHMETIC_OP_MEDIAN: Arithmetic on datasets. (line 161) * GAL_ARITHMETIC_OP_MEDIANVAL: Arithmetic on datasets. (line 144) * GAL_ARITHMETIC_OP_MIN: Arithmetic on datasets. (line 155) * GAL_ARITHMETIC_OP_MINUS: Arithmetic on datasets. (line 65) * GAL_ARITHMETIC_OP_MINVAL: Arithmetic on datasets. (line 138) * GAL_ARITHMETIC_OP_MODULO: Arithmetic on datasets. (line 181) * GAL_ARITHMETIC_OP_MULTIPLY: Arithmetic on datasets. (line 66) * GAL_ARITHMETIC_OP_NE: Arithmetic on datasets. (line 73) * GAL_ARITHMETIC_OP_NOT: Arithmetic on datasets. (line 88) * GAL_ARITHMETIC_OP_NUM: Arithmetic on datasets. (line 157) * GAL_ARITHMETIC_OP_NUMVAL: Arithmetic on datasets. (line 140) * GAL_ARITHMETIC_OP_OR: Arithmetic on datasets. (line 75) * GAL_ARITHMETIC_OP_PLUS: Arithmetic on datasets. (line 64) * GAL_ARITHMETIC_OP_POW: Arithmetic on datasets. (line 170) * GAL_ARITHMETIC_OP_SQRT: Arithmetic on datasets. (line 125) * GAL_ARITHMETIC_OP_STD: Arithmetic on datasets. (line 160) * GAL_ARITHMETIC_OP_STDVAL: Arithmetic on datasets. (line 143) * GAL_ARITHMETIC_OP_SUM: Arithmetic on datasets. (line 158) * GAL_ARITHMETIC_OP_SUMVAL: Arithmetic on datasets. (line 141) * GAL_ARITHMETIC_OP_TO_FLOAT32: Arithmetic on datasets. (line 210) * GAL_ARITHMETIC_OP_TO_FLOAT64: Arithmetic on datasets. (line 211) * GAL_ARITHMETIC_OP_TO_INT16: Arithmetic on datasets. (line 205) * GAL_ARITHMETIC_OP_TO_INT32: Arithmetic on datasets. (line 207) * GAL_ARITHMETIC_OP_TO_INT64: Arithmetic on datasets. (line 209) * GAL_ARITHMETIC_OP_TO_INT8: Arithmetic on datasets. (line 203) * GAL_ARITHMETIC_OP_TO_UINT16: Arithmetic on datasets. (line 204) * GAL_ARITHMETIC_OP_TO_UINT32: Arithmetic on datasets. (line 206) * GAL_ARITHMETIC_OP_TO_UINT64: Arithmetic on datasets. (line 208) * GAL_ARITHMETIC_OP_TO_UINT8: Arithmetic on datasets. (line 202) * GAL_ARITHMETIC_OP_WHERE: Arithmetic on datasets. (line 109) * gal_binary_connected_adjacency_matrix: Binary datasets. (line 139) * gal_binary_connected_components: Binary datasets. (line 114) * gal_binary_dilate: Binary datasets. (line 84) * gal_binary_erode: Binary datasets. (line 62) * gal_binary_fill_holes: Binary datasets. (line 176) * gal_binary_open: Binary datasets. (line 99) * GAL_BINARY_TMP_VALUE: Binary datasets. (line 50) * gal_blank_alloc_write: Library blank values. (line 87) * gal_blank_as_string: Library blank values. (line 142) * gal_blank_flag: Library blank values. (line 126) * GAL_BLANK_FLOAT32: Library blank values. (line 65) * GAL_BLANK_FLOAT64: Library blank values. (line 69) * gal_blank_initialize: Library blank values. (line 94) * GAL_BLANK_INT16: Library blank values. (line 46) * GAL_BLANK_INT32: Library blank values. (line 52) * GAL_BLANK_INT64: Library blank values. (line 58) * GAL_BLANK_INT8: Library blank values. (line 40) * gal_blank_present: Library blank values. (line 102) * gal_blank_remove: Library blank values. (line 133) * GAL_BLANK_SIZE_T: Library blank values. (line 61) * GAL_BLANK_STRING: Library blank values. (line 73) * GAL_BLANK_UINT16: Library blank values. (line 43) * GAL_BLANK_UINT32: Library blank values. (line 49) * GAL_BLANK_UINT64: Library blank values. (line 55) * GAL_BLANK_UINT8: Library blank values. (line 37) * gal_blank_write: Library blank values. (line 79) * gal_box_border_from_center: Bounding box. (line 36) * gal_box_bound_ellipse: Bounding box. (line 22) * gal_box_bound_ellipse_extent: Bounding box. (line 11) * gal_box_overlap: Bounding box. (line 45) * GAL_CONFIG_HAVE_LIBGIT2: Configuration information. (line 25) * GAL_CONFIG_HAVE_PTHREAD_BARRIER: Configuration information. (line 42) * GAL_CONFIG_HAVE_WCSLIB_VERSION: Configuration information. (line 33) * GAL_CONFIG_SIZEOF_LONG: Configuration information. (line 50) * GAL_CONFIG_SIZEOF_SIZE_T: Configuration information. (line 51) * GAL_CONFIG_VERSION: Configuration information. (line 14) * gal_convolve_spatial: Convolution functions. (line 17) * gal_convolve_spatial_correct_ch_edge: Convolution functions. (line 46) * gal_cosmology_age: Cosmology library. (line 18) * gal_cosmology_angular_distance: Cosmology library. (line 46) * gal_cosmology_comoving_volume: Cosmology library. (line 32) * gal_cosmology_critical_density: Cosmology library. (line 39) * gal_cosmology_distance_modulus: Cosmology library. (line 62) * gal_cosmology_luminosity_distance: Cosmology library. (line 54) * gal_cosmology_proper_distance: Cosmology library. (line 25) * gal_cosmology_to_absolute_mag: Cosmology library. (line 69) * gal_data_alloc: Dataset size and allocation. (line 106) * gal_data_array_calloc: Arrays of datasets. (line 20) * gal_data_array_free: Arrays of datasets. (line 36) * gal_data_calloc_array: Dataset size and allocation. (line 64) * gal_data_copy: Copying datasets. (line 18) * gal_data_copy_string_to_number: Copying datasets. (line 65) * gal_data_copy_to_allocated: Copying datasets. (line 44) * gal_data_copy_to_new_type: Copying datasets. (line 24) * gal_data_copy_to_new_type_free: Copying datasets. (line 33) * gal_data_dsize_is_different: Dataset size and allocation. (line 13) * gal_data_free: Dataset size and allocation. (line 129) * gal_data_free_contents: Dataset size and allocation. (line 120) * gal_data_initialize: Dataset size and allocation. (line 71) * gal_data_malloc_array: Dataset size and allocation. (line 44) * gal_data_ptr_dist: Dataset size and allocation. (line 36) * gal_data_ptr_increment: Dataset size and allocation. (line 21) * gal_dimension_add_coords: Dimensions. (line 50) * gal_dimension_coord_to_index: Dimensions. (line 59) * gal_dimension_dist_manhattan: Dimensions. (line 79) * GAL_DIMENSION_FLT_TO_INT: Dimensions. (line 43) * gal_dimension_increment: Dimensions. (line 28) * gal_dimension_index_to_coord: Dimensions. (line 68) * GAL_DIMENSION_NEIGHBOR_OP: Dimensions. (line 87) * gal_dimension_num_neighbors: Dimensions. (line 36) * gal_dimension_total_size: Dimensions. (line 22) * gal_fits_bitpix_to_type: CFITSIO and Gnuastro types. (line 25) * gal_fits_datatype_to_type: CFITSIO and Gnuastro types. (line 49) * gal_fits_hdu_format: FITS HDUs. (line 24) * gal_fits_hdu_num: FITS HDUs. (line 19) * gal_fits_hdu_open: FITS HDUs. (line 30) * gal_fits_hdu_open_format: FITS HDUs. (line 43) * gal_fits_img_info: FITS arrays. (line 11) * gal_fits_img_read: FITS arrays. (line 22) * gal_fits_img_read_kernel: FITS arrays. (line 52) * gal_fits_img_read_to_type: FITS arrays. (line 39) * gal_fits_img_write: FITS arrays. (line 75) * gal_fits_img_write_corr_wcs_str: FITS arrays. (line 97) * gal_fits_img_write_to_ptr: FITS arrays. (line 66) * gal_fits_img_write_to_type: FITS arrays. (line 83) * gal_fits_io_error: FITS macros errors filenames. (line 14) * gal_fits_key_clean_str_value: FITS header keywords. (line 60) * gal_fits_key_img_blank: FITS header keywords. (line 44) * gal_fits_key_list_add: FITS header keywords. (line 153) * gal_fits_key_list_add_end: FITS header keywords. (line 169) * gal_fits_key_read: FITS header keywords. (line 145) * gal_fits_key_read_from_ptr: FITS header keywords. (line 72) * gal_fits_key_write: FITS header keywords. (line 205) * gal_fits_key_write_filename: FITS header keywords. (line 179) * gal_fits_key_write_version: FITS header keywords. (line 212) * gal_fits_key_write_wcsstr: FITS header keywords. (line 195) * GAL_FITS_MAX_NDIM: FITS macros errors filenames. (line 10) * gal_fits_name_is_fits: FITS macros errors filenames. (line 22) * gal_fits_name_save_as_string: FITS macros errors filenames. (line 37) * gal_fits_open_to_write: FITS HDUs. (line 11) * gal_fits_suffix_is_fits: FITS macros errors filenames. (line 30) * gal_fits_tab_format: FITS tables. (line 22) * gal_fits_tab_info: FITS tables. (line 32) * gal_fits_tab_read: FITS tables. (line 53) * gal_fits_tab_size: FITS tables. (line 15) * gal_fits_tab_write: FITS tables. (line 70) * gal_fits_type_to_bin_tform: CFITSIO and Gnuastro types. (line 37) * gal_fits_type_to_bitpix: CFITSIO and Gnuastro types. (line 31) * gal_fits_type_to_datatype: CFITSIO and Gnuastro types. (line 43) * gal_git_describe: Git wrappers. (line 15) * gal_interpolate_close_neighbors: Interpolation. (line 27) * gal_list_data_add: List of gal_data_t. (line 18) * gal_list_data_add_alloc: List of gal_data_t. (line 33) * gal_list_data_free: List of gal_data_t. (line 60) * gal_list_data_number: List of gal_data_t. (line 55) * gal_list_data_pop: List of gal_data_t. (line 44) * gal_list_data_reverse: List of gal_data_t. (line 49) * gal_list_dosizet_add: Doubly linked ordered list of size_t. (line 40) * gal_list_dosizet_free: Doubly linked ordered list of size_t. (line 73) * gal_list_dosizet_pop_smallest: Doubly linked ordered list of size_t. (line 49) * gal_list_dosizet_print: Doubly linked ordered list of size_t. (line 59) * gal_list_dosizet_to_sizet: Doubly linked ordered list of size_t. (line 66) * gal_list_f32_add: List of float. (line 22) * gal_list_f32_free: List of float. (line 81) * gal_list_f32_number: List of float. (line 41) * gal_list_f32_pop: List of float. (line 33) * gal_list_f32_print: List of float. (line 46) * gal_list_f32_reverse: List of float. (line 63) * gal_list_f32_to_array: List of float. (line 69) * gal_list_f64_add: List of double. (line 24) * gal_list_f64_free: List of double. (line 83) * gal_list_f64_number: List of double. (line 43) * gal_list_f64_pop: List of double. (line 35) * gal_list_f64_print: List of double. (line 48) * gal_list_f64_reverse: List of double. (line 65) * gal_list_f64_to_array: List of double. (line 71) * gal_list_i32_add: List of int32_t. (line 23) * gal_list_i32_free: List of int32_t. (line 83) * gal_list_i32_number: List of int32_t. (line 43) * gal_list_i32_pop: List of int32_t. (line 35) * gal_list_i32_print: List of int32_t. (line 48) * gal_list_i32_reverse: List of int32_t. (line 65) * gal_list_i32_to_array: List of int32_t. (line 71) * gal_list_osizet_add: Ordered list of size_t. (line 28) * gal_list_osizet_pop: Ordered list of size_t. (line 39) * gal_list_osizet_to_sizet_free: Ordered list of size_t. (line 49) * gal_list_sizet_add: List of size_t. (line 34) * gal_list_sizet_free: List of size_t. (line 93) * gal_list_sizet_number: List of size_t. (line 53) * gal_list_sizet_pop: List of size_t. (line 45) * gal_list_sizet_print: List of size_t. (line 58) * gal_list_sizet_reverse: List of size_t. (line 75) * gal_list_sizet_to_array: List of size_t. (line 81) * gal_list_str_add: List of strings. (line 20) * gal_list_str_free: List of strings. (line 70) * gal_list_str_number: List of strings. (line 44) * gal_list_str_pop: List of strings. (line 36) * gal_list_str_print: List of strings. (line 49) * gal_list_str_reverse: List of strings. (line 64) * gal_list_void_add: List of void. (line 31) * gal_list_void_free: List of void. (line 60) * gal_list_void_number: List of void. (line 49) * gal_list_void_pop: List of void. (line 42) * gal_list_void_reverse: List of void. (line 54) * gal_match_coordinates: Matching. (line 14) * gal_permutation_apply: Permutations. (line 43) * gal_permutation_apply_inverse: Permutations. (line 50) * gal_permutation_check: Permutations. (line 37) * gal_polygon_area: Polygons. (line 80) * gal_polygon_clip: Polygons. (line 101) * GAL_POLYGON_MAX_CORNERS: Polygons. (line 17) * gal_polygon_ordered_corners: Polygons. (line 25) * gal_polygon_pin: Polygons. (line 88) * gal_polygon_ppropin: Polygons. (line 95) * GAL_POLYGON_ROUND_ERR: Polygons. (line 20) * gal_qsort_index_arr: Qsort functions. (line 16) * gal_qsort_index_float_decreasing: Qsort functions. (line 21) * gal_qsort_TYPE_decreasing: Qsort functions. (line 57) * gal_qsort_TYPE_increasing: Qsort functions. (line 48) * GAL_STATISTICS_BINS_INVALID: Statistical operations. (line 32) * GAL_STATISTICS_BINS_IRREGULAR: Statistical operations. (line 34) * GAL_STATISTICS_BINS_REGULAR: Statistical operations. (line 33) * gal_statistics_cfp: Statistical operations. (line 258) * gal_statistics_histogram: Statistical operations. (line 247) * gal_statistics_is_sorted: Statistical operations. (line 177) * gal_statistics_maximum: Statistical operations. (line 51) * gal_statistics_mean: Statistical operations. (line 64) * gal_statistics_mean_std: Statistical operations. (line 76) * gal_statistics_median: Statistical operations. (line 89) * gal_statistics_minimum: Statistical operations. (line 44) * gal_statistics_mode: Statistical operations. (line 139) * GAL_STATISTICS_MODE_GOOD_SYM: Statistical operations. (line 20) * gal_statistics_mode_mirror_plots: Statistical operations. (line 163) * gal_statistics_no_blank_sorted: Statistical operations. (line 193) * gal_statistics_number: Statistical operations. (line 38) * gal_statistics_quantile: Statistical operations. (line 110) * gal_statistics_quantile_function: Statistical operations. (line 129) * gal_statistics_quantile_function_index: Statistical operations. (line 119) * gal_statistics_quantile_index: Statistical operations. (line 103) * gal_statistics_regular_bins: Statistical operations. (line 203) * gal_statistics_sigma_clip: Statistical operations. (line 279) * GAL_STATISTICS_SIG_CLIP_MAX_CONVERGE: Statistical operations. (line 15) * GAL_STATISTICS_SORTED_DECREASING: Statistical operations. (line 28) * GAL_STATISTICS_SORTED_INCREASING: Statistical operations. (line 27) * GAL_STATISTICS_SORTED_NOT: Statistical operations. (line 26) * gal_statistics_sort_decreasing: Statistical operations. (line 188) * gal_statistics_sort_increasing: Statistical operations. (line 183) * gal_statistics_std: Statistical operations. (line 70) * gal_statistics_sum: Statistical operations. (line 58) * gal_table_comments_add_intro: Table input output. (line 141) * GAL_TABLE_DEF_PRECISION_DBL: Table input output. (line 30) * GAL_TABLE_DEF_PRECISION_FLT: Table input output. (line 29) * GAL_TABLE_DEF_PRECISION_INT: Table input output. (line 28) * GAL_TABLE_DEF_WIDTH_DBL: Table input output. (line 27) * GAL_TABLE_DEF_WIDTH_FLT: Table input output. (line 26) * GAL_TABLE_DEF_WIDTH_INT: Table input output. (line 24) * GAL_TABLE_DEF_WIDTH_LINT: Table input output. (line 25) * GAL_TABLE_DEF_WIDTH_STR: Table input output. (line 23) * GAL_TABLE_DISPLAY_FMT_DECIMAL: Table input output. (line 39) * GAL_TABLE_DISPLAY_FMT_EXP: Table input output. (line 44) * GAL_TABLE_DISPLAY_FMT_FLOAT: Table input output. (line 43) * GAL_TABLE_DISPLAY_FMT_GENERAL: Table input output. (line 45) * GAL_TABLE_DISPLAY_FMT_HEX: Table input output. (line 42) * GAL_TABLE_DISPLAY_FMT_OCTAL: Table input output. (line 41) * GAL_TABLE_DISPLAY_FMT_STRING: Table input output. (line 38) * GAL_TABLE_DISPLAY_FMT_UDECIMAL: Table input output. (line 40) * GAL_TABLE_FORMAT_AFITS: Table input output. (line 67) * GAL_TABLE_FORMAT_BFITS: Table input output. (line 68) * GAL_TABLE_FORMAT_INVALID: Table input output. (line 65) * GAL_TABLE_FORMAT_TXT: Table input output. (line 66) * gal_table_info: Table input output. (line 83) * gal_table_print_info: Table input output. (line 102) * gal_table_read: Table input output. (line 111) * GAL_TABLE_SEARCH_COMMENT: Table input output. (line 76) * GAL_TABLE_SEARCH_INVALID: Table input output. (line 73) * GAL_TABLE_SEARCH_NAME: Table input output. (line 74) * GAL_TABLE_SEARCH_UNIT: Table input output. (line 75) * gal_table_write: Table input output. (line 158) * gal_table_write_log: Table input output. (line 178) * gal_threads_attr_barrier_init: Gnuastro's thread related functions. (line 60) * gal_threads_dist_in_threads: Gnuastro's thread related functions. (line 73) * gal_threads_number: Gnuastro's thread related functions. (line 40) * gal_threads_spin_off: Gnuastro's thread related functions. (line 49) * gal_tile_block: Independent tiles. (line 78) * gal_tile_block_blank_flag: Independent tiles. (line 161) * gal_tile_block_check_tiles: Independent tiles. (line 139) * gal_tile_block_increment: Independent tiles. (line 88) * gal_tile_block_relative_to_other: Independent tiles. (line 152) * gal_tile_block_write_const_value: Independent tiles. (line 104) * gal_tile_full: Tile grid. (line 51) * gal_tile_full_free_contents: Tile grid. (line 242) * gal_tile_full_id_from_coord: Tile grid. (line 233) * gal_tile_full_permutation: Tile grid. (line 152) * gal_tile_full_sanity_check: Tile grid. (line 117) * gal_tile_full_two_layers: Tile grid. (line 126) * gal_tile_full_values_smooth: Tile grid. (line 222) * gal_tile_full_values_write: Tile grid. (line 205) * GAL_TILE_PARSE_OPERATE: Independent tiles. (line 169) * gal_tile_series_from_minmax: Independent tiles. (line 58) * gal_tile_start_coord: Independent tiles. (line 14) * gal_tile_start_end_coord: Independent tiles. (line 22) * gal_tile_start_end_ind_inclusive: Independent tiles. (line 41) * gal_txt_image_read: Text files. (line 79) * GAL_TXT_LINESTAT_BLANK: Text files. (line 27) * GAL_TXT_LINESTAT_COMMENT: Text files. (line 28) * GAL_TXT_LINESTAT_DATAROW: Text files. (line 29) * GAL_TXT_LINESTAT_INVALID: Text files. (line 26) * gal_txt_line_stat: Text files. (line 36) * gal_txt_table_info: Text files. (line 43) * gal_txt_table_read: Text files. (line 62) * gal_txt_write: Text files. (line 88) * GAL_TYPE_BIT: Library data types. (line 44) * gal_type_bit_string: Library data types. (line 187) * GAL_TYPE_COMPLEX32: Library data types. (line 96) * GAL_TYPE_COMPLEX64: Library data types. (line 101) * GAL_TYPE_FLOAT32: Library data types. (line 88) * GAL_TYPE_FLOAT64: Library data types. (line 92) * gal_type_from_name: Library data types. (line 137) * gal_type_from_string: Library data types. (line 227) * GAL_TYPE_INT16: Library data types. (line 60) * GAL_TYPE_INT32: Library data types. (line 68) * GAL_TYPE_INT64: Library data types. (line 76) * GAL_TYPE_INT8: Library data types. (line 52) * GAL_TYPE_INVALID: Library data types. (line 40) * gal_type_is_list: Library data types. (line 176) * GAL_TYPE_LONG: Library data types. (line 84) * gal_type_max: Library data types. (line 161) * gal_type_min: Library data types. (line 146) * gal_type_name: Library data types. (line 124) * gal_type_out: Library data types. (line 181) * gal_type_sizeof: Library data types. (line 117) * GAL_TYPE_SIZE_T: Library data types. (line 80) * GAL_TYPE_STRING: Library data types. (line 106) * gal_type_string_to_number: Library data types. (line 258) * GAL_TYPE_STRLL: Library data types. (line 109) * gal_type_to_string: Library data types. (line 209) * GAL_TYPE_UINT16: Library data types. (line 56) * GAL_TYPE_UINT32: Library data types. (line 64) * GAL_TYPE_UINT64: Library data types. (line 72) * GAL_TYPE_UINT8: Library data types. (line 48) * gal_wcs_angular_distance_deg: World Coordinate System. (line 103) * gal_wcs_copy: World Coordinate System. (line 54) * gal_wcs_decompose_pc_cdelt: World Coordinate System. (line 84) * gal_wcs_img_to_world: World Coordinate System. (line 157) * gal_wcs_on_tile: World Coordinate System. (line 59) * gal_wcs_pixel_area_arcsec2: World Coordinate System. (line 128) * gal_wcs_pixel_scale: World Coordinate System. (line 121) * gal_wcs_read: World Coordinate System. (line 45) * gal_wcs_read_fitsptr: World Coordinate System. (line 13) * gal_wcs_warp_matrix: World Coordinate System. (line 74) * gal_wcs_world_to_img: World Coordinate System. (line 136) * pthread_barrierattr_t: Implementation of pthread_barrier. (line 22) * pthread_barrier_destroy: Implementation of pthread_barrier. (line 43) * pthread_barrier_init: Implementation of pthread_barrier. (line 28) * pthread_barrier_t: Implementation of pthread_barrier. (line 25) * pthread_barrier_wait: Implementation of pthread_barrier. (line 36) Index ***** [index] * Menu: * $HOME: Current directory and User wide. (line 6) * $HOME/.local/etc/: Current directory and User wide. (line 6) * --: Operating mode options. (line 11) * --cite: Operating mode options. (line 55) * --config=STR: Operating mode options. (line 94) * --disable-guide-message: Gnuastro configure options. (line 39) * --disable-progname: Gnuastro configure options. (line 20) * --dontdelete: Input output options. (line 61) * --enable-gnulibcheck: Gnuastro configure options. (line 26) * --enable-gnulibcheck <1>: Known issues. (line 34) * --enable-guide-message=no: Gnuastro configure options. (line 40) * --enable-progname: Gnuastro configure options. (line 12) * --enable-progname=no: Gnuastro configure options. (line 21) * --enable-reentrant: CFITSIO. (line 13) * --hdu=STR/INT: Input output options. (line 10) * --help: Arguments and options. (line 24) * --help <1>: Operating mode options. (line 27) * --help <2>: --help. (line 6) * --help output customization: --help. (line 55) * --ignorecase: Input output options. (line 36) * --keepinputdir: Input output options. (line 68) * --keepinputdir <1>: Automatic output. (line 13) * --lastconfig: Operating mode options. (line 138) * --log: Operating mode options. (line 210) * --numthreads: Configuration files. (line 15) * --numthreads <1>: Multi-threaded operations. (line 16) * --numthreads=INT: Operating mode options. (line 217) * --onlyversion=STR: Operating mode options. (line 150) * --output: Configuration files. (line 15) * --output=STR: Input output options. (line 48) * --prefix: Installation directory. (line 6) * --printparams: Options. (line 64) * --printparams <1>: Operating mode options. (line 72) * --program-prefix: Executable names. (line 50) * --program-suffix: Executable names. (line 50) * --program-transform-name: Executable names. (line 50) * --quiet: Operating mode options. (line 46) * --searchin=STR: Input output options. (line 29) * --setdirconf: Operating mode options. (line 109) * --setdirconf <1>: Current directory and User wide. (line 16) * --setusrconf: Operating mode options. (line 133) * --setusrconf <1>: Current directory and User wide. (line 16) * --tableformat=STR: Input output options. (line 81) * --type=STR: Input output options. (line 54) * --usage: Arguments and options. (line 24) * --usage <1>: Operating mode options. (line 21) * --usage <2>: --usage. (line 6) * --version: Operating mode options. (line 38) * --without-pgplot: WCSLIB. (line 16) * -?: Operating mode options. (line 26) * -D: Input output options. (line 60) * -h STR/INT: Input output options. (line 9) * -I: Input output options. (line 35) * -K: Input output options. (line 67) * -mecube (ds9): Viewing multiextension FITS images. (line 15) * -N INT: Operating mode options. (line 216) * -o STR: Input output options. (line 47) * -P: Operating mode options. (line 71) * -q: Operating mode options. (line 45) * -S: Operating mode options. (line 108) * -s STR: Input output options. (line 28) * -T STR: Input output options. (line 53) * -t STR: Input output options. (line 80) * -U: Operating mode options. (line 132) * -V: Operating mode options. (line 37) * ./.gnuastro/: Current directory and User wide. (line 6) * ./configure: Configuring. (line 6) * ./configure <1>: Installation directory. (line 70) * ./configure options: Gnuastro configure options. (line 6) * .bashrc: --help. (line 65) * .bashrc <1>: Generating random numbers. (line 62) * .desktop: Viewing multiextension FITS images. (line 35) * 32-bit: Configuration information. (line 50) * 64-bit: Configuration information. (line 50) * A4 paper size: A4 print book. (line 6) * A4 print book: A4 print book. (line 6) * ACS: Warp. (line 53) * Additions to Gnuastro: Suggest new feature. (line 6) * Adjacency matrix: Binary datasets. (line 143) * Adobe systems: Recognized file formats. (line 49) * ADU: Flux Brightness and magnitude. (line 6) * ADU <1>: Instrumental noise. (line 19) * Advanced camera for surveys: Warp. (line 53) * Advanced Camera for Surveys: Warping basics. (line 51) * Affine Transformation: Warping basics. (line 85) * Albert. A. Michelson: Science and its tools. (line 134) * Amplifier: Tessellation. (line 54) * Announcements: Announcements. (line 6) * Anonymous bug submission: Report a bug. (line 84) * Anscombe F. J.: Science and its tools. (line 24) * Anscombe’s quartet: Science and its tools. (line 32) * ANSI C: Why C. (line 15) * Aperture blurring: Sigma clipping. (line 22) * Aperture photometry: MakeCatalog. (line 42) * Aperture photometry <1>: Invoking astmkcatalog. (line 53) * Argp argument parser: --help. (line 55) * Argp argument parser <1>: Mandatory source code files. (line 69) * ARGP_HELP_FMT: --help. (line 55) * args.h: Mandatory source code files. (line 68) * Arguments to programs: Arguments and options. (line 6) * Array: Linked lists. (line 6) * ASCII plot: Invoking aststatistics. (line 109) * ASCII table, FITS: Recognized table formats. (line 19) * ASCII85 encoding: Invoking astconvertt. (line 106) * astprogname: Naming convention. (line 15) * Astronomical data format: Recognized file formats. (line 10) * Astronomical data suffixes: Arguments. (line 22) * Astronomical Magnitude system: Flux Brightness and magnitude. (line 28) * Asynchronous thread allocation: Hubble visually checks and classifies his catalog. (line 72) * Asynchronous thread allocation <1>: Invoking astcrop. (line 60) * Atmosphere: Convolve. (line 25) * Atmosphere blurring: Sigma clipping. (line 22) * authors-cite.h: Mandatory source code files. (line 147) * Auto-complete in the shell: Executable names. (line 14) * Automatic configuration file writing: Configuration file format. (line 33) * Automatic output file names: Automatic output. (line 6) * Automatically created build files: Bootstrapping. (line 6) * Available number of threads: Multi-threaded operations. (line 16) * Average: Statistical operations. (line 64) * Average, weighted: Convolve. (line 6) * AWK: General program usage tutorial. (line 961) * AWK <1>: Table. (line 31) * AWK <2>: Invoking asttable. (line 76) * AWK <3>: Invoking astarithmetic. (line 141) * AWK <4>: Invoking aststatistics. (line 156) * AWK <5>: Table input output. (line 120) * Axis ratio: Defining an ellipse. (line 6) * Background flux: Sky value definition. (line 18) * Background flux <1>: Photon counting noise. (line 46) * Background flux gradients: Photon counting noise. (line 61) * Background pixels: Detection options. (line 35) * Backup: Configure and build in RAM. (line 15) * Best use of CPU threads: A note on threads. (line 6) * Bi-linear interpolation: Resampling. (line 21) * Bias current: Tessellation. (line 54) * Bicubic interpolation: Resampling. (line 21) * Bin width, histogram: Histogram and Cumulative Frequency Plot. (line 21) * Binary datasets: Binary datasets. (line 6) * Binary image: Recognized file formats. (line 72) * Binary image <1>: Detection options. (line 35) * Binary table, FITS: Recognized table formats. (line 54) * Bit: Numeric data types. (line 6) * bit-32: Configuration information. (line 50) * bit-64: Configuration information. (line 50) * Bitwise Or: Arithmetic on datasets. (line 40) * Black and white image: Recognized file formats. (line 72) * blank color channel: Recognized file formats. (line 95) * Blank data: Generic data container. (line 147) * Blank pixel: Blank pixels. (line 6) * Blank pixel <1>: Arithmetic operators. (line 245) * Blur image: Convolve. (line 25) * Blur image <1>: PSF. (line 17) * Blurring: Sigma clipping. (line 22) * Book formats: Getting help. (line 6) * Bootstrapping: Bootstrapping. (line 6) * Border on an image: Invoking astconvertt. (line 85) * Breadth first search: Defining an ellipse. (line 35) * Breadth first search <1>: Binary datasets. (line 118) * Brightness: Galaxies. (line 11) * Brightness <1>: Flux Brightness and magnitude. (line 13) * Brightness <2>: Profile magnitude. (line 6) * Buffers (Emacs): Coding conventions. (line 41) * Bug: Report a bug. (line 6) * Bug <1>: Gnuastro project webpage. (line 6) * Bug reporting: Report a bug. (line 16) * Bug tracker: Report a bug. (line 97) * bug-gnuastro@gnu.org: Report a bug. (line 78) * Build: Quick start. (line 6) * Build individual profiles: MakeProfiles output dataset. (line 125) * Build tree: Test scripts. (line 25) * Building from source: Mandatory dependencies. (line 13) * Byte: Numeric data types. (line 15) * C Pre-Processor: Invoking astbuildprog. (line 57) * C programming language: Why C. (line 6) * C++ programming language: Why C. (line 6) * C, plotting: PGPLOT. (line 6) * C99: Dataset size and allocation. (line 54) * C: restrict: Generic data container. (line 60) * Cache, system: A note on threads. (line 29) * Camera: Resampling. (line 6) * CANDELS: Quantifying measurement limits. (line 69) * CCD: Tessellation. (line 54) * CCD <1>: Warp. (line 53) * Central management: Gnuastro project webpage. (line 6) * CFITSIO: CFITSIO. (line 6) * CFITSIO <1>: FITS files. (line 6) * CFITSIO version on outputs: Output headers. (line 6) * Change converted pixel values: Invoking astconvertt. (line 134) * Channel: Tessellation. (line 65) * Charge-coupled device: Warp. (line 53) * Check: Quick start. (line 6) * Check center of crop: Crop options. (line 196) * Checking detection algorithms: MakeProfiles. (line 6) * Checking tests: Tests. (line 6) * Citation information: Mandatory source code files. (line 148) * CLI: command-line user interface: Command-line interface. (line 6) * CLI: repeating operations: Command-line interface. (line 52) * Clump magnitude limit: Quantifying measurement limits. (line 6) * CMYK: Color. (line 6) * Colorspace: Color. (line 6) * Colorspace, gray-scale: Color. (line 6) * Colorspace, transformation: Color. (line 28) * Command-line arguments: Arguments and options. (line 6) * Command-line help: Getting help. (line 13) * Command-line options: Arguments and options. (line 6) * Command-line scroll: --help. (line 27) * Command-line searching text: --help. (line 47) * Command-line token separation: Command-line. (line 12) * Command-line user interface: Command-line interface. (line 6) * Command-line, long outputs: --help. (line 22) * Command-line, viewing full book: Info. (line 6) * Comments: Sufi simulates a detection. (line 324) * Commutative property: Merging multiple warpings. (line 6) * Comoving distance: Distance on a 2D curved space. (line 173) * Compare Moffat and Gaussian: PSF. (line 66) * Compare Poisson and Gaussian: Photon counting noise. (line 33) * Compile: Quick start. (line 6) * Compiled PostScript: Recognized file formats. (line 49) * Compiling from source: Mandatory dependencies. (line 13) * Completeness: Quantifying measurement limits. (line 111) * Complex numbers: Invoking astconvolve. (line 68) * Compression quality in JPEG: Invoking astconvertt. (line 122) * Configuration file directories: Configuration file precedence. (line 6) * Configuration file format: Configuration file format. (line 11) * Configuration file precedence: Configuration file precedence. (line 6) * Configuration file suffix: Configuration file format. (line 6) * Configuration files: Options. (line 92) * Configuration files <1>: Configuration files. (line 6) * Configuration files, system wide: System wide. (line 6) * Configuration files, writing: Configuration file format. (line 33) * Configuration, not finding library: Known issues. (line 11) * Configure options: Configuring. (line 12) * Configure options particular to Gnuastro: Gnuastro configure options. (line 6) * Configuring: Configuring. (line 6) * Connected components: Binary datasets. (line 118) * Connectivity: Binary datasets. (line 13) * Convenient book formats: Getting help. (line 6) * Convention for program source: Program source. (line 6) * Converting data formats: ConvertType. (line 6) * Converting image formats: ConvertType. (line 6) * ConvertType (astconvertt): ConvertType. (line 6) * Convex Hull: Polygons. (line 57) * Convolution: Convolve. (line 6) * Convolution <1>: Convolution process. (line 24) * Convolution <2>: PSF. (line 17) * Convolution kernel: FITS arrays. (line 52) * Cookbook: Tutorials. (line 6) * Coordinate transformation: Warping basics. (line 6) * Coordinates, homogeneous: Warping basics. (line 63) * Copyright: Your rights. (line 12) * Correlated noise: Quantifying measurement limits. (line 206) * Correlation: Convolution process. (line 24) * Cosmic ray removal: Sky value definition. (line 24) * Cosmic rays: Convolve. (line 25) * Cosmic rays <1>: Warp. (line 36) * Cosmic rays <2>: Sigma clipping. (line 22) * Cosmic rays <3>: Sky value definition. (line 17) * Cosmic rays <4>: Quantifying signal in a tile. (line 63) * COSMOS survey: Crop. (line 13) * Counting error: Photon counting noise. (line 6) * Counting from zero.: Options. (line 110) * Counts: Flux Brightness and magnitude. (line 6) * Counts <1>: Instrumental noise. (line 19) * CPPFLAGS: Known issues. (line 46) * CPPFLAGS <1>: Headers. (line 153) * CPU threads: Multi-threaded operations. (line 6) * CPU threads <1>: MakeProfiles profile settings. (line 161) * CPU threads, number: Configuration files. (line 15) * CPU threads, set number: Operating mode options. (line 216) * CPU, using all threads: Multi-threaded operations. (line 6) * Crop (astcrop): Crop. (line 6) * Crop a given section of image: Crop section syntax. (line 6) * Crop part of image: Crop. (line 6) * Crop section format: Crop section syntax. (line 25) * Cumulative Frequency Plot: Histogram and Cumulative Frequency Plot. (line 31) * Customize --help output: --help. (line 55) * Customize executable names: Executable names. (line 28) * Customizing installation: Configuring. (line 12) * Data: Quantifying signal in a tile. (line 6) * Data format conversion: ConvertType. (line 6) * Data structures: Headers. (line 89) * Data type: Generic data container. (line 69) * Data’s depth: Quantifying measurement limits. (line 51) * Dataset: binary: Binary datasets. (line 6) * de Vaucouleur profile: Galaxies. (line 11) * Debug: Invoking astbuildprog. (line 113) * Debugging: Building and debugging. (line 39) * Default executable search directory: Installation directory. (line 70) * Default library search directory: Installation directory. (line 159) * Default option values: Options. (line 92) * Default option values <1>: Configuration files. (line 6) * Define section to crop: Crop section syntax. (line 12) * Dependencies, Gnuastro: Mandatory dependencies. (line 6) * Depth: Quantifying measurement limits. (line 6) * Detached threads: Gnuastro's thread related functions. (line 64) * Detection: Convolve. (line 25) * Detection <1>: NoiseChisel. (line 6) * Detections false: Quantifying measurement limits. (line 123) * Detector: Resampling. (line 6) * Development packages: Known issues. (line 11) * Diffraction limited: PSF. (line 6) * Dilation: Binary datasets. (line 92) * Directory, install: Installation directory. (line 144) * Discrete Fourier transform: Invoking astconvolve. (line 46) * Distortion, optical: Warp. (line 47) * Distribution mode: Sky value misconceptions. (line 20) * Douglas Rushkoff: Science and its tools. (line 50) * Drizzle: Resampling. (line 48) * Dynamic libraries: Installation directory. (line 189) * Dynamic linking: Linking. (line 55) * Edges, image: Resampling. (line 32) * Edwin Hubble: Hubble visually checks and classifies his catalog. (line 6) * Effective radius: Galaxies. (line 11) * Efficient use of CPU threads: A note on threads. (line 6) * Ellipse: Defining an ellipse. (line 6) * Elliptical distance: Defining an ellipse. (line 28) * Elliptical galaxies: Hubble visually checks and classifies his catalog. (line 113) * Emacs buffers: Coding conventions. (line 41) * Encapsulated PostScript: Recognized file formats. (line 41) * Environment: Installation directory. (line 50) * Environment variable, HOME: Installation directory. (line 63) * Environment variables: Installation directory. (line 37) * Environment variables <1>: Installation directory. (line 50) * Environment variables <2>: Generating random numbers. (line 26) * eog: Hubble visually checks and classifies his catalog. (line 100) * EPS: Recognized file formats. (line 41) * Erosion: NoiseChisel. (line 45) * Erosion <1>: Detection options. (line 100) * Erosion <2>: Binary datasets. (line 77) * Error, floating point round-off: Invoking astconvolve. (line 82) * etc: Configuration files. (line 6) * Exact area resampling: Resampling. (line 48) * Executable names: Executable names. (line 6) * Extreme Deep Field survey: General program usage tutorial. (line 6) * Eye of GNOME: Hubble visually checks and classifies his catalog. (line 100) * False detections: Quantifying measurement limits. (line 123) * Feature request: Gnuastro project webpage. (line 6) * Feature requests: Suggest new feature. (line 6) * File I/O: Configure and build in RAM. (line 6) * File operations: Data containers. (line 6) * File system Hierarchy Standard: Configuration files. (line 6) * file systems, tmpfs: Configure and build in RAM. (line 23) * first-in-first-out: Linked lists. (line 47) * first-in-first-out <1>: FITS header keywords. (line 23) * FITS: FITS files. (line 6) * FITS image viewer: SAO ds9. (line 6) * FITS standard: CFITSIO. (line 6) * FITS standard <1>: Invoking astwarp. (line 66) * FITS standard <2>: Generic data container. (line 77) * FITS Tables: Recognized table formats. (line 19) * Fitting: Modeling and fittings. (line 6) * Flip coordinates: Warping basics. (line 30) * Floating point error: Measuring elliptical parameters. (line 47) * Floating point round-off error: Invoking astconvolve. (line 82) * FLT: Options. (line 38) * Flux: Flux Brightness and magnitude. (line 13) * Flux to magnitude conversion: Flux Brightness and magnitude. (line 28) * Foreground pixels: Detection options. (line 35) * FORTRAN: Generic data container. (line 77) * Fourier spectrum: Invoking astconvolve. (line 68) * Free software: Your rights. (line 12) * Free Software Foundation: Contributing to Gnuastro. (line 16) * FSF: Contributing to Gnuastro. (line 16) * Full Width at Half Maximum: PSF. (line 27) * Function gradient over pixel area: Sampling from a function. (line 16) * Function groups: Coding conventions. (line 153) * Functions for user interface: Mandatory source code files. (line 102) * FWHM: PSF. (line 27) * Gain: Flux Brightness and magnitude. (line 6) * Gain <1>: Instrumental noise. (line 19) * Galaxy profiles: Galaxies. (line 6) * Galileo, G.: Science and its tools. (line 104) * Gaussian: Invoking astnoisechisel. (line 23) * Gaussian <1>: Invoking astmkcatalog. (line 31) * Gaussian distribution: Quantifying signal in a tile. (line 6) * Gaussian distribution <1>: PSF. (line 37) * Gaussian FWHM: PSF. (line 50) * GCC: Summary and example on libraries. (line 30) * Gedit: Hubble visually checks and classifies his catalog. (line 143) * Gedit <1>: Sufi simulates a detection. (line 335) * General file operations: Data containers. (line 6) * Generalized de Vaucouleur profile: Galaxies. (line 6) * Git: Optional dependencies. (line 52) * Git <1>: Version controlled source. (line 6) * Git <2>: Table input output. (line 141) * Git <3>: Git wrappers. (line 6) * GNOME: General program usage tutorial. (line 661) * GNOME 2: Viewing multiextension FITS images. (line 58) * GNOME 3: Command-line interface. (line 18) * GNOME 3 <1>: Viewing multiextension FITS images. (line 30) * GNU Astronomy Utilities (Gnuastro): Introduction. (line 6) * GNU Autoconf: Bootstrapping dependencies. (line 61) * GNU Autoconf <1>: Bootstrapping. (line 63) * GNU Autoconf <2>: Synchronizing. (line 21) * GNU Autoconf <3>: Configuring. (line 21) * GNU Autoconf <4>: Building and debugging. (line 6) * GNU Autoconf Archive: Bootstrapping dependencies. (line 65) * GNU Autoconf Archive <1>: Bootstrapping. (line 6) * GNU Automake: Bootstrapping dependencies. (line 55) * GNU Automake <1>: Bootstrapping. (line 63) * GNU Automake <2>: Building and debugging. (line 6) * GNU AWK: General program usage tutorial. (line 272) * GNU AWK <1>: General program usage tutorial. (line 902) * GNU AWK <2>: Table. (line 31) * GNU AWK <3>: Invoking asttable. (line 35) * GNU AWK <4>: Invoking asttable. (line 76) * GNU AWK <5>: Invoking astarithmetic. (line 141) * GNU AWK <6>: Invoking aststatistics. (line 156) * GNU AWK <7>: Table input output. (line 120) * GNU Bash: Command-line interface. (line 52) * GNU Bash <1>: Hubble visually checks and classifies his catalog. (line 113) * GNU Bash <2>: Installation directory. (line 110) * GNU Bash <3>: Installation directory. (line 120) * GNU Bash <4>: Keyword manipulation. (line 80) * GNU Bash <5>: Program design philosophy. (line 27) * GNU Binutils: Linking. (line 16) * GNU build system: Mandatory dependencies. (line 6) * GNU build system <1>: Bootstrapping. (line 63) * GNU build system <2>: Installation directory. (line 144) * GNU build system <3>: Configure and build in RAM. (line 34) * GNU build system <4>: Headers. (line 153) * GNU build system <5>: Headers. (line 162) * GNU build system <6>: Building and debugging. (line 6) * GNU C library: New to GNU/Linux?. (line 19) * GNU C library <1>: Bootstrapping dependencies. (line 28) * GNU C library <2>: Bootstrapping. (line 63) * GNU C library <3>: Gnuastro configure options. (line 27) * GNU C library <4>: Configure and build in RAM. (line 34) * GNU C library <5>: Info. (line 28) * GNU C library <6>: Adding new columns to MakeCatalog. (line 53) * GNU C library <7>: Linking. (line 101) * GNU C library <8>: Coding conventions. (line 83) * GNU C library <9>: Mandatory source code files. (line 69) * GNU coding standards: Introduction. (line 6) * GNU coding standards <1>: Coding conventions. (line 6) * GNU coding standards <2>: Coding conventions. (line 132) * GNU Compiler Collection: New to GNU/Linux?. (line 19) * GNU Compiler Collection <1>: Summary and example on libraries. (line 30) * GNU Compiler Collection <2>: Invoking astbuildprog. (line 96) * GNU Compiler Collection <3>: Coding conventions. (line 34) * GNU Coreutils: Multi-threaded operations. (line 6) * GNU Coreutils <1>: Program design philosophy. (line 18) * GNU CPP: Invoking astbuildprog. (line 57) * GNU Emacs: Command-line interface. (line 75) * GNU Emacs <1>: Hubble visually checks and classifies his catalog. (line 113) * GNU Emacs <2>: Hubble visually checks and classifies his catalog. (line 143) * GNU Emacs <3>: Sufi simulates a detection. (line 335) * GNU Emacs <4>: Configure and build in RAM. (line 50) * GNU Emacs <5>: Info. (line 28) * GNU Emacs <6>: Coding conventions. (line 146) * GNU Emacs <7>: Coding conventions. (line 153) * GNU Emacs <8>: Coding conventions. (line 192) * GNU Free Documentation License: Your rights. (line 40) * GNU Free Documentation License <1>: GNU Free Doc. License. (line 6) * GNU General Public License: Your rights. (line 40) * GNU Grep: General program usage tutorial. (line 628) * GNU Grep <1>: General program usage tutorial. (line 638) * GNU Grep <2>: --help. (line 47) * GNU Grep <3>: Keyword manipulation. (line 46) * GNU Grep <4>: CosmicCalculator specific calculations. (line 32) * GNU help2man: Bootstrapping dependencies. (line 77) * GNU Info: General program usage tutorial. (line 47) * GNU Info <1>: Info. (line 6) * GNU Libtool: Optional dependencies. (line 23) * GNU Libtool <1>: Bootstrapping dependencies. (line 71) * GNU Libtool <2>: Bootstrapping. (line 63) * GNU Libtool <3>: Known issues. (line 76) * GNU Libtool <4>: Linking. (line 6) * GNU Libtool <5>: Linking. (line 55) * GNU Libtool <6>: Linking. (line 130) * GNU Libtool <7>: BuildProgram. (line 15) * GNU Libtool <8>: Invoking astbuildprog. (line 75) * GNU Libtool <9>: Building and debugging. (line 6) * GNU Make: How to run simultaneous operations. (line 57) * GNU Make <1>: Invoking astbuildprog. (line 49) * GNU Parallel: Hubble visually checks and classifies his catalog. (line 86) * GNU Parallel <1>: How to run simultaneous operations. (line 15) * GNU Portability Library (Gnulib): Bootstrapping dependencies. (line 28) * GNU Portability Library (Gnulib) <1>: Bootstrapping. (line 6) * GNU Portability Library (Gnulib) <2>: Gnuastro configure options. (line 27) * GNU Portability Library (Gnulib) <3>: Known issues. (line 34) * GNU Portability Library (Gnulib) <4>: Coding conventions. (line 83) * GNU Savannah: Gnuastro project webpage. (line 6) * GNU Scientific Library: GNU Scientific Library. (line 6) * GNU Scientific Library <1>: Generating random numbers. (line 26) * GNU Scientific Library <2>: Permutations. (line 16) * GNU software documentation: Info. (line 22) * GNU style options: Options. (line 6) * GNU Tar: Quick start. (line 6) * GNU Tar <1>: Quick start. (line 15) * GNU Texinfo: Your rights. (line 6) * GNU Texinfo <1>: Bootstrapping. (line 63) * GNU Texinfo <2>: A4 print book. (line 13) * GNU Texinfo <3>: Known issues. (line 71) * GNU/Linux: New to GNU/Linux?. (line 19) * Gnuastro coding convention: Coding conventions. (line 6) * Gnuastro common options: Common options. (line 6) * Gnuastro major version number: GNU Astronomy Utilities 1.0. (line 6) * Gnuastro program structure convention: Program source. (line 6) * Gnuastro project page: Report a bug. (line 84) * Gnuastro test scripts: Test scripts. (line 6) * Gnulib: Program design philosophy. (line 6) * Gnulib: GNU Portability Library: Bootstrapping dependencies. (line 28) * Gnulib: GNU Portability Library <1>: Bootstrapping. (line 6) * Gnulib: GNU Portability Library <2>: Gnuastro configure options. (line 27) * Gnulib: GNU Portability Library <3>: Known issues. (line 34) * Gnulib: GNU Portability Library <4>: Coding conventions. (line 83) * GPL Ghostscript: Optional dependencies. (line 10) * GPL Ghostscript <1>: Optional dependencies. (line 71) * GPL Ghostscript <2>: Known issues. (line 62) * GPL Ghostscript <3>: Recognized file formats. (line 86) * Gradient over pixel area: Sampling from a function. (line 16) * Gradients in background flux: Photon counting noise. (line 61) * Graphic user interface: Command-line interface. (line 6) * Gravitational lensing: Warp. (line 13) * Grayscale: Color. (line 6) * Groups of similar functions: Coding conventions. (line 153) * GUI: graphic user interface: Command-line interface. (line 6) * GUI: repeating operations: Command-line interface. (line 43) * Gzip: Quick start. (line 15) * Gzip <1>: Release tarball. (line 37) * Gérard de Vaucouleurs: Galaxies. (line 11) * Halted program: Report a bug. (line 6) * HDD: Configure and build in RAM. (line 12) * HDU: Arguments and options. (line 42) * HDU <1>: Input output options. (line 9) * HDU <2>: Invoking astfits. (line 38) * Header data unit: Arguments and options. (line 42) * Header data unit <1>: Input output options. (line 9) * Header file: Coding conventions. (line 67) * Help: Getting help. (line 6) * help-gnuastro mailing list: help-gnuastro mailing list. (line 6) * help-gnuastro@gnu.org: help-gnuastro mailing list. (line 13) * Hexadecimal encoding: Invoking astconvertt. (line 106) * Histogram: Histogram and Cumulative Frequency Plot. (line 6) * Histogram <1>: Sky value misconceptions. (line 20) * HOME: Installation directory. (line 63) * HOME/.local/: Installation directory. (line 63) * Homogeneous coordinates: Warping basics. (line 63) * Homography: Warping basics. (line 93) * HST: General program usage tutorial. (line 6) * Hubble Space Telescope: General program usage tutorial. (line 6) * Hubble Space Telescope <1>: Tessellation. (line 54) * Hubble Space Telescope <2>: Crop. (line 13) * Hubble Space Telescope <3>: Warp. (line 53) * Hubble Space Telescope <4>: Warping basics. (line 51) * Hyper Suprime-Cam: Tessellation. (line 54) * Image: Color. (line 6) * Image blurring: PSF. (line 17) * Image edges: Resampling. (line 32) * Image format conversion: ConvertType. (line 6) * Image mosaic: Crop. (line 13) * Image mosaic <1>: Warp. (line 29) * Image noise: Noise basics. (line 6) * Image tiles: Crop. (line 13) * Image transformations: MakeProfiles. (line 41) * ImageMagick: Bootstrapping dependencies. (line 113) * Imaging surveys: Crop. (line 13) * Immediate neighbors: Binary datasets. (line 13) * Inconsistent results: Report a bug. (line 6) * Individual profiles: MakeProfiles output dataset. (line 125) * info-gnuastro@gnu.org: Synchronizing. (line 21) * INFOPATH: Installation directory. (line 159) * Input/Output, file: Configure and build in RAM. (line 6) * Inside-out construction: Defining an ellipse. (line 35) * Inside-out construction <1>: Sampling from a function. (line 44) * Install directory: Installation directory. (line 144) * Install with no super-user access: Installation directory. (line 6) * Installation: Installation. (line 6) * Installation, customizing: Configuring. (line 12) * Installed help methods: Getting help. (line 22) * Instrumental noise: Instrumental noise. (line 6) * INT: Options. (line 35) * Integer, Signed: Numeric data types. (line 15) * Integration over pixel: Sampling from a function. (line 16) * Integration to infinity: Profile magnitude. (line 15) * Internal default value: Configuration files. (line 15) * Internally stored option value: Multi-threaded operations. (line 16) * Interpolation: Resampling. (line 21) * Interpolation, bi-linear: Resampling. (line 21) * Interpolation, bicubic: Resampling. (line 21) * Intervals, histogram: Histogram and Cumulative Frequency Plot. (line 21) * ISO C90: Why C. (line 15) * Issue: Gnuastro project webpage. (line 6) * Jaynes E. T.: Science and its tools. (line 152) * JPEG compression quality: Invoking astconvertt. (line 122) * JPEG format: Optional dependencies. (line 60) * JPEG format <1>: Recognized file formats. (line 23) * Ken Thomson: Science and its tools. (line 115) * Kernel, convolution: Convolve. (line 6) * Kernel, convolution <1>: FITS arrays. (line 52) * Kernighan, Brian: Why C. (line 15) * Labeling: NoiseChisel. (line 6) * Large astronomical images: Crop. (line 6) * last-in-first-out: Linked lists. (line 47) * last-in-first-out <1>: FITS header keywords. (line 23) * LaTeX: Bootstrapping dependencies. (line 81) * LaTeX <1>: Recognized file formats. (line 60) * LaTeX <2>: Program design philosophy. (line 27) * Lawrence Livermore National Laboratory: Multithreaded programming. (line 20) * LDFLAGS: Known issues. (line 24) * LD_LIBRARY_PATH: Installation directory. (line 159) * LD_LIBRARY_PATH <1>: Known issues. (line 52) * LD_LIBRARY_PATH <2>: PGPLOT. (line 62) * Learning GNU Info: Info. (line 22) * Lensing simulations: MakeProfiles. (line 41) * less: --help. (line 33) * libgit2: Optional dependencies. (line 52) * libgit2 <1>: Git wrappers. (line 6) * libjpeg: Optional dependencies. (line 60) * Library search directory: Installation directory. (line 159) * Library: shared: Linking. (line 55) * Limit, object/clump magnitude: Quantifying measurement limits. (line 6) * Linear spatial filtering: Convolution process. (line 16) * Linked list: Linked lists. (line 6) * Linked list <1>: FITS header keywords. (line 23) * Linking: dynamic: Linking. (line 55) * Linking: Static: Linking. (line 31) * Linux: New to GNU/Linux?. (line 19) * Linux kernel: Configure and build in RAM. (line 34) * Long option abbreviation: Options. (line 64) * Long outputs: --help. (line 22) * Lord Kelvin: Science and its tools. (line 128) * Low level programming: Why C. (line 89) * Luminosity: Flux Brightness and magnitude. (line 13) * Lzip: Quick start. (line 15) * Lzip <1>: Release tarball. (line 37) * Macro: Headers. (line 89) * Magnitude zero-point: Flux Brightness and magnitude. (line 28) * Magnitude, object/clump detection limit: Quantifying measurement limits. (line 6) * Magnitude, upper limit: Quantifying measurement limits. (line 192) * Magnitudes from flux: Flux Brightness and magnitude. (line 28) * Mailing list archives: Report a bug. (line 78) * Mailing list archives <1>: help-gnuastro mailing list. (line 13) * Mailing list: bug-gnuastro: Report a bug. (line 78) * Mailing list: bug-gnuastro <1>: Gnuastro project webpage. (line 19) * Mailing list: gnuastro-commits: Developing mailing lists. (line 37) * Mailing list: gnuastro-commits <1>: Commit guidelines. (line 34) * Mailing list: gnuastro-commits <2>: Commit guidelines. (line 50) * Mailing list: gnuastro-commits <3>: Commit guidelines. (line 72) * Mailing list: gnuastro-devel: Gnuastro project webpage. (line 58) * Mailing list: gnuastro-devel <1>: Developing mailing lists. (line 13) * Mailing list: help-gnuastro: help-gnuastro mailing list. (line 6) * Mailing list: info-gnuastro: Version numbering. (line 6) * Mailing list: info-gnuastro <1>: Announcements. (line 6) * Mailing list: info-gnuastro <2>: Synchronizing. (line 21) * main function: Mandatory source code files. (line 19) * Main parameters C structure: Mandatory source code files. (line 30) * main.c: Mandatory source code files. (line 18) * main.h: Mandatory source code files. (line 29) * Major version number: Version numbering. (line 6) * Make: How to run simultaneous operations. (line 38) * make check: Tests. (line 6) * MakeProfiles (astmkprof): MakeProfiles. (line 6) * Making a distribution package: Developer's checklist. (line 24) * Making profiles pixel by pixel: Defining an ellipse. (line 35) * Man pages: Man pages. (line 6) * Management hub: Gnuastro project webpage. (line 6) * Mandatory arguments: Arguments and options. (line 24) * Mandatory arguments <1>: --usage. (line 6) * MANPATH: Installation directory. (line 159) * Mathematical morphology: Binary datasets. (line 77) * Matplotlib, Python: Program design philosophy. (line 27) * Matplotlib, Python <1>: PGPLOT. (line 14) * Matrix: Warping basics. (line 17) * Matrix multiplication: Merging multiple warpings. (line 6) * Matrix, adjacency: Binary datasets. (line 143) * Maximum: Statistical operations. (line 51) * Mean: Statistical operations. (line 64) * Median: Quantifying signal in a tile. (line 28) * Median <1>: Statistical operations. (line 89) * Meta-data: Fits. (line 20) * Metacharacters: Command-line. (line 12) * Metacharacters on the command-line: Arguments and options. (line 35) * Michelson, Albert. A.: Science and its tools. (line 134) * Minimum: Statistical operations. (line 44) * Minor version number: Version numbering. (line 6) * Mixing pixel values: Convolve. (line 25) * Mixing pixel values <1>: Resampling. (line 6) * mock.fits: Tests. (line 6) * Mode: Quantifying signal in a tile. (line 28) * Mode of a distribution: Sky value misconceptions. (line 20) * Modeling: Modeling and fittings. (line 6) * Modeling stars: Stars. (line 6) * Modifying print book: A4 print book. (line 6) * Modularity: Review of library fundamentals. (line 18) * Moffat beta: PSF. (line 59) * Moffat function: PSF. (line 53) * Moffat FWHM: PSF. (line 64) * Moments: Measuring elliptical parameters. (line 15) * Monte carlo integration: Sampling from a function. (line 26) * Mosaicing: Crop. (line 13) * Mosaicing <1>: Warp. (line 29) * Multi-threaded programs: Multi-threaded operations. (line 6) * Multiextension FITS: Viewing multiextension FITS images. (line 6) * Multiple file opening, reentrancy: CFITSIO. (line 13) * Multiplication, Matrix: Warping basics. (line 17) * Multiplication, matrix: Merging multiple warpings. (line 6) * Multithreaded programming: Multithreaded programming. (line 6) * Möbius, August. F.: Warping basics. (line 63) * Names of executables: Executable names. (line 6) * Names, customize: Executable names. (line 28) * Names, programs: Naming convention. (line 6) * NaN: Gnuastro text table format. (line 73) * NaN <1>: Arithmetic operators. (line 98) * NaN <2>: Invoking astwarp. (line 174) * NaN <3>: Invoking aststatistics. (line 435) * NaN <4>: Detection options. (line 87) * NaN <5>: MakeCatalog general settings. (line 46) * NaN <6>: Library blank values. (line 17) * NaN <7>: Library blank values. (line 29) * NaN <8>: Library blank values. (line 65) * NaN <9>: Library blank values. (line 69) * NaN <10>: FITS arrays. (line 52) * Navigating source files: Program source. (line 6) * Necessary parameters: Configuration files. (line 6) * Neighborhood: Convolve. (line 6) * Neighbors, immediate: Binary datasets. (line 13) * No access to super-user install: Installation directory. (line 6) * Noise: Quantifying signal in a tile. (line 6) * Noise <1>: MakeNoise. (line 6) * Noise <2>: Noise basics. (line 6) * Noise simulation: Photon counting noise. (line 67) * Noise, instrumental: Instrumental noise. (line 6) * Non-commutative operations: Merging multiple warpings. (line 6) * Normalizing histogram: Histogram and Cumulative Frequency Plot. (line 21) * nproc: Multi-threaded operations. (line 6) * Number: Statistical operations. (line 38) * Number of CPU threads to use: Operating mode options. (line 216) * Number of CPU threads to use <1>: Configuration files. (line 15) * Number of threads available: Multi-threaded operations. (line 16) * Number, version: Version numbering. (line 6) * Numbers, complex: Invoking astconvolve. (line 68) * Numbers, psudo-random: Generating random numbers. (line 14) * Numbers, random: Generating random numbers. (line 6) * Object magnitude limit: Quantifying measurement limits. (line 6) * Object oriented programming: Why C. (line 27) * On/Off options: Options. (line 25) * Online help: Getting help. (line 13) * Opening (Mathematical morphology): Binary datasets. (line 107) * Opening multiextension FITS: Viewing multiextension FITS images. (line 6) * OpenMP: Multithreaded programming. (line 32) * Operations on files: Data containers. (line 6) * Operations, non-commutative: Merging multiple warpings. (line 6) * Operator, structure de-reference: Mandatory source code files. (line 56) * Optical distortion: Warp. (line 47) * Optimization: Invoking astbuildprog. (line 96) * Optimization <1>: Building and debugging. (line 39) * Optimization flag: Coding conventions. (line 34) * Option values: Options. (line 47) * Optional and mandatory tokens: --usage. (line 6) * Options: Invoking astarithmetic. (line 127) * Options common to all programs: Common options. (line 6) * Options to programs: Arguments and options. (line 6) * Options, abbreviation: Options. (line 64) * Options, GNU style: Options. (line 6) * Options, on/off: Options. (line 25) * Options, repeated: Options. (line 72) * Options, short (-) and long (--): Options. (line 6) * Order in search directory: Installation directory. (line 204) * Output file names, automatic: Automatic output. (line 6) * Output FITS headers: Output headers. (line 6) * Output, wrong: Report a bug. (line 6) * Oversample: Sufi simulates a detection. (line 169) * Oversampling: Oversampling. (line 6) * p: Mandatory source code files. (line 45) * Package managers: Mandatory dependencies. (line 13) * Paper size, A4: A4 print book. (line 6) * Paper size, US letter: A4 print book. (line 6) * Parametric PSFs: PSF. (line 27) * PATH: Installation directory. (line 70) * PDF: Recognized file formats. (line 49) * permutation: Permutations. (line 6) * PGFplots in TeX or LaTeX: Program design philosophy. (line 27) * PGFplots in TeX or LaTeX <1>: PGPLOT. (line 14) * PGPLOT: PGPLOT. (line 6) * Phase angle: Invoking astconvolve. (line 68) * photo-electrons: Sky value definition. (line 48) * Photoelectrons: Resampling. (line 6) * Photometry, aperture: MakeCatalog. (line 42) * Photometry, aperture <1>: Invoking astmkcatalog. (line 53) * Photon counting noise: Photon counting noise. (line 6) * Picture element: Resampling. (line 6) * Pipe: --help. (line 33) * Pixel: Resampling. (line 6) * Pixel by pixel making of profiles: Defining an ellipse. (line 35) * Pixel mixing: Convolve. (line 25) * Pixel mixing <1>: Resampling. (line 6) * Pixel mixing <2>: Resampling. (line 48) * Pixelated graphics: Recognized file formats. (line 23) * Pixels: Color. (line 6) * Plain text: Recognized file formats. (line 100) * Plotting directly in C: PGPLOT. (line 6) * PNG standard: Color. (line 40) * Point pixels: Resampling. (line 21) * Point source: PSF. (line 6) * Point Spread Function: PSF. (line 6) * Poisson distribution: Photon counting noise. (line 23) * Portable Document format: Recognized file formats. (line 49) * Position angle: Measuring elliptical parameters. (line 132) * Position angle <1>: Defining an ellipse. (line 6) * POSIX threads: Implementation of pthread_barrier. (line 6) * POSIX Threads: Gnuastro's thread related functions. (line 6) * POSIX threads library: Multithreaded programming. (line 20) * Post-fix notation: Reverse polish notation. (line 6) * Postage stamp images: Crop. (line 6) * PostScript: Recognized file formats. (line 41) * PostScript vs. PDF: Recognized file formats. (line 49) * Pre-Processor: Headers. (line 6) * Pre-processor macros: Headers. (line 89) * Precedence, configuration files: Configuration file precedence. (line 6) * prefix/etc/: System wide. (line 6) * Primary colors: Color. (line 6) * printf: Table input output. (line 31) * Probability density function: Histogram and Cumulative Frequency Plot. (line 21) * Probability density function <1>: Sky value misconceptions. (line 20) * Probability density function <2>: Photon counting noise. (line 16) * Profiles, galaxies: Galaxies. (line 6) * progname.c, progname.h: Mandatory source code files. (line 122) * prognameparams: Mandatory source code files. (line 30) * Program crashing: Report a bug. (line 6) * Program names: Naming convention. (line 6) * Program structure convention: Program source. (line 6) * Programming, low level: Why C. (line 89) * ProgramName: Naming convention. (line 15) * Projective transformation: Warping basics. (line 93) * Proper distance: Distance on a 2D curved space. (line 142) * PSF: PSF. (line 6) * PSF image size: PSF. (line 17) * PSF over-sample: Oversampling. (line 12) * PSF width: PSF. (line 27) * PSF, Moffat compared Gaussian: PSF. (line 66) * Psudo-random numbers: Generating random numbers. (line 14) * pthread: Multi-threaded operations. (line 6) * pthread_barrier: Implementation of pthread_barrier. (line 6) * Public domain: Your rights. (line 12) * Purity: Quantifying measurement limits. (line 123) * Puzzle solving scientist: Science and its tools. (line 141) * Python Matplotlib: Program design philosophy. (line 27) * Python Matplotlib <1>: PGPLOT. (line 14) * Python programming language: Why C. (line 6) * Quality of compression in JPEG: Invoking astconvertt. (line 122) * Quantile: Invoking aststatistics. (line 98) * Quantile <1>: Detection options. (line 35) * Quantile <2>: Statistical operations. (line 103) * Radial profile on ellipse: Defining an ellipse. (line 15) * Radius, effective: Galaxies. (line 11) * Random numbers: Generating random numbers. (line 6) * Raster graphics: Recognized file formats. (line 23) * Readout noise: Instrumental noise. (line 6) * Redirection of output: --help. (line 22) * Redirection of output <1>: --help. (line 42) * Reentrancy, multiple file opening: CFITSIO. (line 13) * Remembering options: Getting help. (line 6) * Remote operation: Command-line interface. (line 91) * Removing ast from executables: Executable names. (line 70) * Repeated options: Options. (line 72) * Report a bug: Gnuastro project webpage. (line 6) * Reproducibility: Upper-limit magnitude settings. (line 14) * Reproducible bug reports: Report a bug. (line 64) * Reproducible results: Command-line interface. (line 52) * Resampling: Resampling. (line 6) * Resource heavy operations: Command-line interface. (line 83) * restrict: Generic data container. (line 60) * Results, wrong: Report a bug. (line 6) * Reverse Polish Notation: Reverse polish notation. (line 6) * RGB: Color. (line 6) * Ritchie, Dennis: Why C. (line 15) * Root access, not possible: Installation directory. (line 6) * Root parameter structure: Mandatory source code files. (line 30) * Rotation of coordinates: Warping basics. (line 17) * Round-off error: Invoking astconvolve. (line 82) * Round-off error <1>: Polygons. (line 21) * Sampling: Resampling. (line 6) * Sampling <1>: Sampling from a function. (line 6) * SAO ds9: Crop options. (line 122) * SAO ds9 <1>: SAO ds9. (line 6) * Save output to file: --help. (line 42) * Saving binary image: Recognized file formats. (line 72) * Scaling: Warping basics. (line 6) * Scientist, puzzle solver: Science and its tools. (line 141) * Scripts, startup: Installation directory. (line 110) * Scroll command-line: --help. (line 27) * Search directory for executables: Installation directory. (line 70) * Search directory order: Installation directory. (line 204) * Searching text: --help. (line 47) * Second moment: Measuring elliptical parameters. (line 25) * Section of an image: Crop. (line 6) * Secure shell: Command-line interface. (line 91) * SED, stream editor: Executable names. (line 60) * Seed, psudo-random numbers: Generating random numbers. (line 14) * Segmentation: NoiseChisel. (line 6) * Separating tokens on the command-line: Command-line. (line 12) * Setting output file names automatically: Automatic output. (line 6) * Setting PATH: Installation directory. (line 70) * Shared library: Linking. (line 55) * Shared library versioning: Linking. (line 115) * Shear: Warping basics. (line 38) * Shell: Command-line interface. (line 6) * Shell auto-complete: Executable names. (line 14) * Shell script: GNU Astronomy Utilities 1.0. (line 12) * Shell variables: Installation directory. (line 37) * and : --help. (line 27) * sigma-clipping: Sky value misconceptions. (line 27) * Signal: Quantifying signal in a tile. (line 6) * Signal to noise ratio: Warp. (line 20) * Signal to noise ratio <1>: Resampling. (line 21) * Signed integer: Numeric data types. (line 15) * Simulating noise: Photon counting noise. (line 67) * Simultaneous multithreading: Multi-threaded operations. (line 6) * Single channel CMYK: Color. (line 40) * size_t: Ordered list of size_t. (line 16) * size_t <1>: Doubly linked ordered list of size_t. (line 14) * Skewed Poisson distribution: Photon counting noise. (line 26) * Sky: Sky value. (line 6) * Sky value: Sky value definition. (line 6) * Sky value <1>: Sky value definition. (line 34) * Sky value <2>: Photon counting noise. (line 46) * Software bug: Report a bug. (line 6) * Source code building: Mandatory dependencies. (line 13) * Source code compilation: Mandatory dependencies. (line 13) * Source file navigation: Program source. (line 6) * Source tree: Test scripts. (line 25) * Source, uncompress: Quick start. (line 6) * Spectrum, Fourier: Invoking astconvolve. (line 68) * Spiral galaxies: Hubble visually checks and classifies his catalog. (line 113) * Spread of a point source: PSF. (line 6) * SSD: Configure and build in RAM. (line 12) * SSH: Command-line interface. (line 91) * Standard deviation: Measuring elliptical parameters. (line 35) * Standard deviation <1>: Statistical operations. (line 70) * Standard, FITS: Generic data container. (line 77) * Stars, modeling: Stars. (line 6) * Startup scripts: Installation directory. (line 110) * Startup scripts <1>: Generating random numbers. (line 62) * Static document description format: Recognized file formats. (line 49) * Static linking: Linking. (line 31) * Statistical analysis: Science and its tools. (line 32) * Stitch multiple images: Crop. (line 20) * STR: Options. (line 43) * Stream editor, SED: Executable names. (line 60) * Stroustrup, Bjarne: Science and its tools. (line 115) * Stroustrup, Bjarne <1>: Why C. (line 15) * Structure de-reference operator: Mandatory source code files. (line 56) * Structures: Headers. (line 89) * Subaru Telescope: Tessellation. (line 54) * Submit new tracker item: Report a bug. (line 84) * Suffixes, astronomical data: Arguments. (line 22) * Suffixes, EPS format: Recognized file formats. (line 81) * Suffixes, JPEG images: Recognized file formats. (line 36) * Suffixes, PDF format: Recognized file formats. (line 86) * Suffixes, plain text: Recognized file formats. (line 100) * Sum: Statistical operations. (line 58) * Sum for total flux: Profile magnitude. (line 6) * Superuser, not possible: Installation directory. (line 6) * Support request manager: Report a bug. (line 84) * Surface brightness: Quantifying measurement limits. (line 29) * Symbolic link: Executable names. (line 38) * System Cache: A note on threads. (line 29) * System wide configuration files: System wide. (line 6) * Sérsic index: Galaxies. (line 11) * Sérsic profile: Galaxies. (line 6) * Sérsic, J. L.: Galaxies. (line 11) * Tables FITS: Recognized table formats. (line 19) * Tabs are evil: Coding conventions. (line 151) * Task tracker: Report a bug. (line 97) * Test: Quick start. (line 6) * Test scripts: Test scripts. (line 6) * Tests, only one passes: Known issues. (line 52) * Tests, running: Tests. (line 6) * tests/during-dev.sh: Building and debugging. (line 23) * TeX: Known issues. (line 71) * TeX <1>: Recognized file formats. (line 60) * TeX Live: Bootstrapping dependencies. (line 81) * Threads, CPU: MakeProfiles profile settings. (line 161) * Thresholding: Binary datasets. (line 6) * Tilde expansion as option values: Options. (line 101) * tmpfs file system: Configure and build in RAM. (line 23) * tmpfs-config-make: Building and debugging. (line 18) * tmpfs-config-make <1>: Test scripts. (line 25) * Token separation: Command-line. (line 12) * Top processing source file: Mandatory source code files. (line 123) * Top root structure: Mandatory source code files. (line 30) * Tracker: Report a bug. (line 97) * Tracker <1>: Gnuastro project webpage. (line 6) * Trailing space: Coding conventions. (line 146) * Transform image: MakeProfiles. (line 41) * Transformation, affine: Warping basics. (line 85) * Transformation, projective: Warping basics. (line 93) * Truncation radius: Profile magnitude. (line 6) * Tutorial: Tutorials. (line 6) * Type: Numeric data types. (line 6) * ui.c: Mandatory source code files. (line 101) * ui.h: Mandatory source code files. (line 85) * Uncompress source: Quick start. (line 6) * Undetected objects: Photon counting noise. (line 46) * Unsigned integer: Numeric data types. (line 15) * Upper limit magnitude: Quantifying measurement limits. (line 192) * US letter paper size: A4 print book. (line 6) * Usage pattern: --usage. (line 6) * User interface functions: Mandatory source code files. (line 102) * Using CPU threads: Multi-threaded operations. (line 6) * Using multiple CPU cores: Multi-threaded operations. (line 6) * Using multiple threads: A note on threads. (line 6) * Values to options: Options. (line 47) * Variance: Measuring elliptical parameters. (line 25) * Variation of background flux: Photon counting noise. (line 61) * Vector graphics: Recognized file formats. (line 41) * Version control: Report a bug. (line 27) * Version control <1>: Version controlled source. (line 6) * Version control systems: Optional dependencies. (line 52) * Version number: Version numbering. (line 6) * Versioning: Shared library: Linking. (line 115) * Viewing trackers: Report a bug. (line 97) * Virtual console: Command-line interface. (line 75) * void *: Generic data container. (line 50) * Wall-clock time: A note on threads. (line 19) * WCS: WCSLIB. (line 6) * WCSLIB: WCSLIB. (line 6) * WCSLIB <1>: Invoking astwarp. (line 205) * Weighted average: Convolve. (line 6) * WFC3: Warp. (line 53) * White space character: Configuration file format. (line 11) * Wide Field Camera 3: Warp. (line 53) * Wide Field Camera 3 <1>: Warping basics. (line 51) * William Thomson: Science and its tools. (line 128) * World Coordinate System: WCSLIB. (line 6) * World Coordinate System <1>: Invoking astwarp. (line 205) * Writing configuration files: Configuration file format. (line 33) * Wrong output: Report a bug. (line 6) * Wrong results: Report a bug. (line 6) * XDF: Quantifying measurement limits. (line 69) * XDF survey: General program usage tutorial. (line 6) * Zero-point magnitude: Flux Brightness and magnitude. (line 42) gnuastro-0.5/doc/gnuastro.info-40000644000175000017500000106370113217220436013576 00000000000000This is gnuastro.info, produced by makeinfo version 6.5 from gnuastro.texi. This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro’s library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Library blank values, Next: Library data container, Prev: Library data types, Up: Gnuastro library 10.3.4 Library blank values (‘blank.h’) --------------------------------------- When the position of an element in a dataset is important (for example a pixel in an image), a place-holder is necessary for the element if we don’t have a value to fill it with (for example the CCD cannot read those pixels). We cannot simply shift all the other pixels to fill in the one we have no value for. In other cases, it often occurs that the field of sky that you are studying is not a clean rectangle to nicely fit into the boundaries of an image. You need a way to separate the pixels outside your scientific field from those inside it. Blank values act as these place holders in a dataset. They have no usable value but they have a position. Every type needs a corresponding blank value (see *note Numeric data types:: and *note Library data types::). Floating point types have a unique value identified by IEEE known as Not-a-Number (or NaN) which is a unique value that is recognized by the compiler. However, integer and string types don’t have any standard value. For integers, in Gnuastro we take an extremum of the given type: for signed types (that allow negatives), the minimum possible value is used as blank and for unsigned types (that only accept positives), the maximum possible value is used. To be generic and easy to read/write we define a macro for these blank values and strongly encourage you only use these, and never make any assumption on the value of a type’s blank value. The IEEE NaN blank value type is defined to fail on any comparison, so if you are dealing with floating point types, you cannot use equality (a NaN will _not_ be equal to a NaN). If you know your dataset if floating point, you can use the ‘isnan’ function in C’s ‘math.h’ header. For a description of numeric data types see *note Numeric data types::. For the constants identifying integers, please see *note Library data types::. -- Global integer: GAL_BLANK_UINT8 Blank value for an unsigned, 8-bit integer. -- Global integer: GAL_BLANK_INT8 Blank value for a signed, 8-bit integer. -- Global integer: GAL_BLANK_UINT16 Blank value for an unsigned, 16-bit integer. -- Global integer: GAL_BLANK_INT16 Blank value for a signed, 16-bit integer. -- Global integer: GAL_BLANK_UINT32 Blank value for an unsigned, 32-bit integer. -- Global integer: GAL_BLANK_INT32 Blank value for a signed, 32-bit integer. -- Global integer: GAL_BLANK_UINT64 Blank value for an unsigned, 64-bit integer. -- Global integer: GAL_BLANK_INT64 Blank value for a signed, 64-bit integer. -- Global integer: GAL_BLANK_SIZE_T Blank value for ‘size_t’ type (‘uint32_t’ or ‘uint64_t’ in 32-bit or 64-bit systems). -- Global integer: GAL_BLANK_FLOAT32 Blank value for a single precision, 32-bit floating point type (IEEE NaN value). -- Global integer: GAL_BLANK_FLOAT64 Blank value for a double precision, 64-bit floating point type (IEEE NaN value). -- Global integer: GAL_BLANK_STRING Blank value for string types (this is itself a string, it isn’t the ‘NULL’ pointer). The functions below can be used to work with blank pixels. -- Function: void gal_blank_write (void ‘*pointer’, uint8_t ‘type’) Write the blank value for the given ‘type’ into the space that ‘pointer’ points to. This can be used when the space is already allocated (for example one element in an array or a statically allocated variable). -- Function: void * gal_blank_alloc_write (uint8_t ‘type’) Allocate the space required to keep the blank for the given data type ‘type’, write the blank value into it and return the pointer to it. -- Function: void gal_blank_initialize (gal_data_t ‘*input’) Initialize all the elements in the ‘input’ dataset to the blank value that corresponds to its type. If ‘input’ is a tile over a larger dataset, only the region that the tile covers will be set to blank. -- Function: int gal_blank_present (gal_data_t ‘*input’, int ‘updateflag’) Return 1 if the dataset has a blank value and zero if it doesn’t. Before checking the dataset, this function will look at ‘input’’s flags. If the ‘GAL_DATA_FLAG_HASBLANK’ or ‘GAL_DATA_FLAG_DONT_CHECK_ZERO’ bits of ‘input->flag’ are set to 1, this function will not do any check and will just use the information in the flags. This can greatly speed up processing when a dataset needs to be checked multiple times. If you want to re-check a dataset which has non-zero flags, then explicitly set the appropriate flag to zero before calling this function. When there are no other flags, you can just set ‘input->flags’ to zero, otherwise you can use this expression: input->flags &= ~(GAL_DATA_FLAG_HASBLANK | GAL_DATA_FLAG_USE_ZERO); When ‘updateflags’ is zero, this function has no side-effects on the dataset: it will not toggle the flags. When the dataset’s flags were not used and ‘updateflags’ is non-zero, this function will set the flags appropriately to avoid having to re-check the dataset in future calls. -- Function: gal_data_t * gal_blank_flag (gal_data_t ‘*input’) Create a dataset of the the same size as the input, but with an ‘uint8_t’ type that has a value of 1 for data that are blank and 0 for those that aren’t. -- Function: void gal_blank_remove (gal_data_t ‘*input’) Remove blank elements from a dataset, convert it to a 1D dataset, and adjust the size properly (the number of non-blank elements). In practice this function doesn’t ‘realloc’ the input array, it just shifts the blank elements to the end and adjusts the size elements of the ‘gal_data_t’, see *note Generic data container::. -- Function: char * gal_blank_as_string (uint8_t ‘type’, int ‘width’) Write the blank value for the given data type ‘type’ into a string and return it. The space for the string is dynamically allocated so it must be freed after you are done with it.  File: gnuastro.info, Node: Library data container, Next: Dimensions, Prev: Library blank values, Up: Gnuastro library 10.3.5 Data container (‘data.h’) -------------------------------- Astronomical datasets have various dimensions, for example 1D spectra or table columns, 2D images, or 3D Integral field data cubes. Datasets can also have various numeric data types, depending on the operation/purpose, for example processed images are in commonly in floating point, but their mask images are integers using bit-wise flags to identify certain classes of special pixels, see *note Numeric data types::). Certain other information about a dataset are also commonly necessary, for example the units of the dataset, the name of the dataset and some comments. To deal with any generic dataset, Gnuastro defines the ‘gal_data_t’ as input or output. * Menu: * Generic data container:: Definition of Gnuastro’s generic container. * Dataset size and allocation:: Functions for size and allocation. * Arrays of datasets:: Functions to help with array of datasets. * Copying datasets:: Functions to copy a dataset to a new one.  File: gnuastro.info, Node: Generic data container, Next: Dataset size and allocation, Prev: Library data container, Up: Library data container 10.3.5.1 Generic data container (‘gal_data_t’) .............................................. To be able to deal with any dataset (various dimensions, numeric data types, units and higher-level structures), Gnuastro defines the ‘gal_data_t’ type which is the input/output container of choice for many of Gnuastro library’s functions. It is defined in ‘gnuastro/data.h’. If you will be using (‘‘# include’’ing) those libraries, you don’t need to include this header explicitly, it is already included by any library header that uses ‘gal_data_t’. -- Type (C ‘struct’): gal_data_t The main container for datasets in Gnuastro. It can host data of any dimensions, with any numeric data type. It is actually a structure, but ‘typedef’’d as a new type to avoid having to write the ‘struct’ before any declaration. The actual structure is shown below which is followed by a description of each element. typedef struct gal_data_t { void *restrict array; /* Basic array information. */ uint8_t type; size_t ndim; size_t *dsize; size_t size; char *mmapname; size_t minmapsize; int nwcs; /* WCS information. */ struct wcsprm *wcs; uint8_t flag; /* Content description. */ int status; char *name; char *unit; char *comment; int disp_fmt; /* For text printing. */ int disp_width; int disp_precision; struct gal_data_t *next; /* For higher-level datasets. */ struct gal_data_t *block; } gal_data_t; The list below contains a description for each ‘gal_data_t’ element. ‘void *restrict array’ This is the pointer to the main array of the dataset containing the raw data (values). All the other elements in this data-structure are actually meta-data enabling us to use/understand the series of values in this array. It must allow data of any type (see *note Numeric data types::), so it is defined as a ‘void *’ pointer. A ‘void *’ array is not directly usable in C, so you have to cast it to proper type before using it, please see *note Library demo - reading a image:: for a demonstration. The ‘restrict’ keyword was formally introduced in C99 and is used to tell the compiler that at any moment only this pointer will modify what it points to (a pixel in an image for example)(1). This extra piece of information can greatly help in compiler optimizations and thus the running time of the program. But older compilers might not have this capability, so at ‘./configure’ time, Gnuastro checks this feature and if the user’s compiler doesn’t support ‘restrict’, it will be removed from this definition. ‘uint8_t type’ A fixed code (integer) used to identify the type of data in ‘array’ (see *note Numeric data types::). For the list of acceptable values to this variable, please see *note Library data types::. ‘size_t ndim’ The dataset’s number of dimensions. ‘size_t *dsize’ The size of the dataset along each dimension. This is an array (with ‘ndim’ elements), of positive integers in row-major order(2) (based on C). When a data file is read into memory with Gnuastro’s libraries, this array is dynamically allocated based on the number of dimensions that the dataset has. It is important to remember that C’s row-major ordering is the opposite of the FITS standard which is in column-major order: in the FITS standard the fastest dimension’s size is specified by ‘NAXIS1’, and slower dimensions follow. The FITS standard was defined mainly based on the FORTRAN language which is the opposite of C’s approach to multi-dimensional arrays (and also starts counting from 1 not 0). Hence if a FITS image has ‘NAXIS1==20’ and ‘NAXIS2==50’, the ‘dsize’ array must be filled with ‘dsize[0]==50’ and ‘dsize[1]==20’. The fastest dimension is the one that is contiguous in memory: to increment by one along that dimension, just go to the next element in the array. As we go to slower dimensions, the number of memory cells we have to skip for an increment along that dimension becomes larger. ‘size_t size’ The total number of elements in the dataset. This is actually a multiplication of all the values in the ‘dsize’ array, so it is not an independent parameter. However, low-level operations with the dataset (irrespective of its dimensions) commonly need this number, so this element is designed to avoid calculating it every time. ‘char *mmapname’ Name of file hosting the ‘mmap’’d contents of ‘array’. If the value of this variable is ‘NULL’, then the contents of ‘array’ are actually stored in RAM, not in a file on the HDD/SSD. See the description of ‘minmapsize’ below for more. If a file is used, it will be kept in the hidden ‘.gnuastro’ directory with a randomly selected name to allow multiple arrays to be kept there at the same time. When ‘gal_data_free’ is called the randomly named file will be deleted. ‘size_t minmapsize’ The minimum size of an array (in bytes) to store the contents of ‘array’ as a file (on the non-volatile HDD/SSD), not in RAM. This can be very useful for large datasets which can be very memory intensive and the user’s RAM might not be sufficient to keep/process it. A random filename is assigned to the array which is available in the ‘mmapname’ element of ‘gal_data_t’ (above), see there for more. ‘minmapsize’ is stored in each ‘gal_data_t’, so it can be passed on to subsequent/derived datasets. See the description of the ‘--minmapsize’ option in *note Processing options:: for more on using this value. ‘nwcs’ The number of WCS coordinate representations (for WCSLIB). ‘struct wcsprm *wcs’ The main WCSLIB structure keeping all the relevant information necessary for WCSLIB to do its processing and convert data-set positions into real-world positions. When it is given a ‘NULL’ value, all possible WCS calculations/measurements will be ignored. ‘uint8_t flag’ Bit-wise flags to describe general properties of the dataset. The number of bytes available in this flag is stored in the ‘GAL_DATA_FLAG_SIZE’ macro. Note that you should use bit-wise operators(3) to check these flags. The currently recognized bits are stored in these macros: ‘GAL_DATA_FLAG_BLANK_CH’ Marking that the dataset has been checked for blank values. Therefore, the value of the bit in ‘GAL_DATA_FLAG_HASBLANK’ is reliable. Without this bit, when a dataset doesn’t have any blank values (and this has been checked), the ‘GAL_DATA_FLAG_HASBLANK’ bit will be zero so a checker has no way to know if this zero is real or if no check has been done yet. ‘GAL_DATA_FLAG_HASBLANK’ This bit has a value of ‘1’ when the given dataset has blank values. If this bit is ‘0’ and ‘GAL_DATA_FLAG_BLANK_CH’ is ‘1’, then the dataset has been checked and it didn’t have any blank values, so there is no more need for further checks. ‘GAL_DATA_FLAG_SORT_CH’ Marking that the dataset is already checked for being sorted or not and thus that the possible ‘0’ values in ‘GAL_DATA_FLAG_SORTED_I’ and ‘GAL_DATA_FLAG_SORTED_D’ are meaningful. ‘GAL_DATA_FLAG_SORTED_I’ This bit has a value of ‘1’ when the given dataset is sorted in an increasing manner. If this bit is ‘0’ and ‘GAL_DATA_FLAG_SORT_CH’ is ‘1’, then the dataset has been checked and wasn’t sorted (increasing), so there is no more need for further checks. ‘GAL_DATA_FLAG_SORTED_D’ This bit has a value of ‘1’ when the given dataset is sorted in a decreasing manner. If this bit is ‘0’ and ‘GAL_DATA_FLAG_SORT_CH’ is ‘1’, then the dataset has been checked and wasn’t sorted (decreasing), so there is no more need for further checks. The macro ‘GAL_DATA_FLAG_MAXFLAG’ contains the largest internally used bit-position. Higher-level flags can be defined with the bit-wise shift operators using this macro to define internal flags for libraries/programs that depend on Gnuastro without causing any possible conflict with the internal flags discussed above or having to check the values manually on every release. ‘int status’ A context-specific status values for this data-structure. This integer will not be set by Gnuastro’s libraries. You can use it keep some additional information about the dataset (with integer constants) depending on your applications. ‘char *name’ The name of the dataset. If the dataset is a multi-dimensional array and read/written as a FITS image, this will be the value in the ‘EXTNAME’ FITS keyword. If the dataset is a one-dimensional table column, this will be the column name. If it is set to ‘NULL’ (by default), it will be ignored. ‘char *unit’ The units of the dataset (for example ‘BUNIT’ in the standard FITS keywords) that will be read from or written to files/tables along with the dataset. If it is set to ‘NULL’ (by default), it will be ignored. ‘char *comment’ Any further explanation about the dataset which will be written to any output file if present. ‘disp_fmt’ Format to use for printing each element of the dataset to a plain text file, the acceptable values to this element are defined in *note Table input output::. Based on C’s ‘printf’ standards. ‘disp_width’ Width of printing each element of the dataset to a plain text file, the acceptable values to this element are defined in *note Table input output::. Based on C’s ‘printf’ standards. ‘disp_precision’ Precision of printing each element of the dataset to a plain text file, the acceptable values to this element are defined in *note Table input output::. Based on C’s ‘printf’ standards. ‘gal_data_t *next’ Through this pointer, you can link a ‘gal_data_t’ with other datasets related datasets, for example the different columns in a dataset each have one ‘gal_data_t’ associate with them and they are linked to each other using this element. There are several functions described below to facilitate using ‘gal_data_t’ as a linked list. See *note Linked lists:: for more on these wonderful high-level constructs. ‘gal_data_t *block’ Pointer to the start of the complete allocated block of memory. When this pointer is not ‘NULL’, the dataset is not treated as a contiguous patch of memory. Rather, it is seen as covering only a portion of the larger patch of memory that ‘block’ points to. See *note Tessellation library:: for a more thorough explanation and functions to help work with tiles that are created from this pointer. ---------- Footnotes ---------- (1) Also see . (2) Also see . (3) See .  File: gnuastro.info, Node: Dataset size and allocation, Next: Arrays of datasets, Prev: Generic data container, Up: Library data container 10.3.5.2 Dataset size and allocation .................................... Gnuastro’s main data container was defined in *note Generic data container::. The functions listed in this section describe the most basic operations on ‘gal_data_t’: those related to the size, pointers, allocation and freeing. These functions are declared in ‘gnuastro/data.h’ which is also visible from the function names (see *note Gnuastro library::). -- Function: int gal_data_dsize_is_different (gal_data_t ‘*first’, gal_data_t ‘*second’) Return ‘1’ (one) if the two datasets don’t have the same size along all dimensions. This function will also return ‘1’ when the number of dimensions of the two datasets are different. -- Function: void * gal_data_ptr_increment (void ‘*pointer’, size_t ‘increment’, uint8_t ‘type’) Return a pointer to an element that is ‘increment’ elements ahead of ‘pointer’, assuming each element has type of ‘type’ (for the type codes, see *note Library data types::). When working with the ‘array’ elements of ‘gal_data_t’, we are actually dealing with ‘void *’ pointers. However, pointer arithmetic doesn’t apply to ‘void *’, because the system doesn’t know how many bytes there are in each element to increment the pointer respectively. This function will use the given ‘type’ to calculate where the incremented element is located in memory. -- Function: size_t gal_data_ptr_dist (void ‘*earlier’, void ‘*later’, uint8_t ‘type’) Return the number of elements between ‘earlier’ and ‘later’ assuming each element has a type defined by ‘type’ (for the type codes, see *note Library data types::). -- Function: void * gal_data_malloc_array (uint8_t ‘type’, size_t ‘size’, const char ‘*funcname’, const char ‘*varname’) Allocate an array of type ‘type’ with ‘size’ elements in RAM (for the type codes, see *note Library data types::). This is effectively just a wrapper around C’s ‘malloc’ function but takes Gnuastro’s integer type codes and will also abort with an error if there the allocation was not successful. When space cannot be allocated, this function will abort the program with a message containing the reason for the failure. ‘funcname’ (name of the function calling this function) and ‘varname’ (name of variable that needs this space) will be used in this error message if they are not ‘NULL’. In most modern compilers, you can use the generic ‘__func__’ variable for ‘funcname’. In this way, you don’t have to manually copy and paste the function name or worry about it changing later (‘__func__’ was standardized in C99). -- Function: void * gal_data_calloc_array (uint8_t ‘type’, size_t ‘size’, const char ‘*funcname’, const char ‘*varname’) Similar to ‘gal_data_malloc_array’, but the space is cleared (set to 0) after allocation. -- Function: void gal_data_initialize (gal_data_t ‘*data’, void ‘*array’, uint8_t ‘type’, size_t ‘ndim’, size_t ‘*dsize’, struct wcsprm ‘*wcs’, int ‘clear’, size_t ‘minmapsize’, char ‘*name’, char ‘*unit’, char ‘*comment’) Initialize the given data structure (‘data’) with all the given values. Note that the raw input ‘gal_data_t’ must already have been allocated before calling this function. For a description of each variable see *note Generic data container::. It will set the values and do the necessary allocations. If they aren’t ‘NULL’, all input arrays (‘dsize’, ‘wcs’, ‘name’, ‘unit’, ‘comment’) are separately copied (allocated) by this function for usage in ‘data’, so you can safely use one value to initialize many datasets or use statically allocated variables in this function call. Once you are done with the dataset, you can clean all the allocated spaces with ‘gal_data_free_contents’. If ‘array’ is not ‘NULL’, it will be directly copied into ‘data->array’ and no new space will be allocated for the array of this dataset, this has many low-level advantages and can be used to work on regions of a dataset instead of the whole allocated array (see the description under ‘block’ in *note Generic data container:: for one example). If the given pointer is not the start of an allocated block of memory or it is used in multiple datasets, be sure to set it to ‘NULL’ (with ‘data->array=NULL’) before cleaning up with ‘gal_data_free_contents’. ‘ndim’ may be zero. In this case no allocation will occur, ‘data->array’ and ‘data->dsize’ will be set to ‘NULL’ and ‘data->size’ will be zero. However (when necessary) ‘dsize’ must not have any zero values (a dimension of length zero is not defined). -- Function: gal_data_t * gal_data_alloc (void ‘*array’, uint8_t ‘type’, size_t ‘ndim’, size_t ‘*dsize’, struct wcsprm ‘*wcs’, int ‘clear’, size_t ‘minmapsize’, char ‘*name’, char ‘*unit’, char ‘*comment’) Dynamically allocate a ‘gal_data_t’ and initialize it will all the given values. See the description of ‘gal_data_initialize’ and *note Generic data container:: for more information. This function will often be the most frequently used because it allocates the ‘gal_data_t’ hosting all the values _and_ initializes it. Once you are done with the dataset, be sure to clean up all the allocated spaces with ‘gal_data_free’. -- Function: void gal_data_free_contents (gal_data_t ‘*data’) Free all the non-‘NULL’ pointers in ‘gal_data_t’. If ‘data’ is actually a tile (‘data->block!=NULL’, see *note Tessellation library::), then ‘tile->array’ is not freed. For a complete description of ‘gal_data_t’ and its contents, see *note Generic data container::. -- Function: void gal_data_free (gal_data_t ‘*data’) Free all the non-‘NULL’ pointers in ‘gal_data_t’, then free the actual data structure.  File: gnuastro.info, Node: Arrays of datasets, Next: Copying datasets, Prev: Dataset size and allocation, Up: Library data container 10.3.5.3 Arrays of datasets ........................... Gnuastro’s generic data container (‘gal_data_t’) is a very versatile structure that can be used in many higher-level contexts. One such higher-level construct is an array of ‘gal_data_t’ structures to simplify the allocation (and later cleaning) of several ‘gal_data_t’s that are related. For example, each column in a table is usually represented by one ‘gal_data_t’ (so it has its own name, numeric data type, units and etc). A table (with many columns) can be seen as an array of ‘gal_data_t’s (when the number of columns is known a-priori). The functions below are defined to create a cleared array of data structures and to free them in the end. These functions are declared in ‘gnuastro/data.h’ which is also visible from the function names (see *note Gnuastro library::). -- Function: gal_data_t * gal_data_array_calloc (size_t ‘size’) Allocate an array of ‘gal_data_t’ with ‘size’ elements. This function will also initialize all the values (‘NULL’ for pointers and 0 for other types). You can use ‘gal_data_initialize’ to fill each element of the array afterwards. The following code snippet is one example of doing this. size_t i; gal_data_t *dataarr; dataarr=gal_data_array_calloc(10); for(i=0;i<10;++i) gal_data_initialize(&dataarr[i], ...); ... gal_data_array_free(dataarr, 10, 1); -- Function: void gal_data_array_free (gal_data_t ‘*dataarr’, size_t ‘num’, int ‘free_array’) Free all the ‘num’ elements within ‘dataarr’ and the actual allocated array. If ‘free_array’ is not zero, then the ‘array’ element of all the datasets will also be freed, see *note Generic data container::.  File: gnuastro.info, Node: Copying datasets, Prev: Arrays of datasets, Up: Library data container 10.3.5.4 Copying datasets ......................... The functions in this section describes Gnuastro’s facilities to copy a given dataset into another. The new dataset can have a different type (including a string), it can be already allocated (in which case only the values will be written into it). In all these cases, if the input dataset is a tile, only the data within the tile are copied. In many of the functions here, it is possible to copy the dataset to a new numeric data type (see *note Numeric data types::. In such cases, Gnuastro’s library is going to use the native conversion by C. So if you are converting to a smaller type, it is up to you to make sure that the values fit into the output type. -- Function: gal_data_t * gal_data_copy (gal_data_t ‘*in’) Return a new dataset that is a copy of ‘in’, all of ‘in’’s meta-data will also copied into the output, except for ‘block’. -- Function: gal_data_t * gal_data_copy_to_new_type (gal_data_t ‘*in’, uint8_t ‘newtype’) Return a copy of the dataset ‘in’, converted to ‘newtype’, see *note Library data types:: for Gnuastro library’s type identifiers. The returned dataset will have all meta-data except their type and ‘block’ equal to the input’s metadata. -- Function: gal_data_t * gal_data_copy_to_new_type_free (gal_data_t ‘*in’, uint8_t ‘newtype’) Return a copy of the dataset ‘in’ that is converted to ‘newtype’ and free the input dataset. See *note Library data types:: for Gnuastro library’s type identifiers. The returned dataset will have all meta-data, except their type, equal to the input’s metadata. This function is similar to ‘gal_data_copy_to_new_type’, except that it will free the input dataset. -- Function: void gal_data_copy_to_allocated (gal_data_t ‘*in’, gal_data_t ‘*out’) Copy the contents of the array in ‘in’ into the already allocated array in ‘out’. The types of the input and output may be different, type conversion will be done internally. When ‘in->size != out->size’ this function will behave as follows: ‘out->size < in->size’ This function won’t re-allocate the necessary space, it will abort with an error, so please check before calling this function. ‘out->size > in->size’ This function will write the values in ‘out->size’ and ‘out->dsize’ from the same values of ‘in’. So if you want to use a pre-allocated space/dataset multiple times with varying input sizes, be sure to reset ‘out->size’ before every call to this function. -- Function: gal_data_t * gal_data_copy_string_to_number (char ‘*string’) Read ‘string’ into the smallest type that can store the value (see *note Numeric data types::). This function is just a wrapper for the ‘gal_type_string_to_number’, but will put the value into a single-element dataset.  File: gnuastro.info, Node: Dimensions, Next: Linked lists, Prev: Library data container, Up: Gnuastro library 10.3.6 Dimensions (‘dimension.h’) --------------------------------- An array is a contiguous region of memory. Hence, at the lowest level, every element of an array just has one single-valued position: the number of elements that lie between it and the first element in the array. This is also known as the _index_ of the element within the array. A dataset’s number of dimensions is high-level abstraction (meta-data) that we project onto that contiguous patch of memory. When the array is interpreted as a one-dimensional dataset, this index is also the _coordinate_ of the element. But once we associate the patch of memory with a higher dimension, there must also be one coordinate for each dimension. The functions and macros in this section provide you with the tools to convert an index into a coordinate and vice-versa along with several other issues for example issues with the neighbors of an element in a multi-dimensional context. -- Function: size_t gal_dimension_total_size (size_t ‘ndim’, size_t ‘*dsize’) Return the total number of elements for a dataset with ‘ndim’ dimensions that has ‘dsize’ elements along each dimension. -- Function: size_t * gal_dimension_increment (size_t ‘ndim’, size_t ‘*dsize’) Return an allocated array that has the number of elements necessary to increment an index along every dimension. For example along the fastest dimension (last element in the ‘dsize’ and returned arrays), the value is ‘1’ (one). -- Function: size_t gal_dimension_num_neighbors (size_t ‘ndim’) The maximum number of neighbors (any connectivity) that a data element can have in ‘ndim’ dimensions. Effectively, this function just returns $3^n-1$ (where $n$ is the number of dimensions). -- Function-like macro: GAL_DIMENSION_FLT_TO_INT (‘FLT’) Calculate the integer pixel position that the floating point ‘FLT’ number belongs to. In the FITS format (and thus in Gnuastro), the center of each pixel is allocated on an integer (not it edge), so the pixel which hosts a floating point number cannot simply be found with internal type conversion. -- Function: void gal_dimension_add_coords (size_t ‘*c1’, size_t ‘*c2’, size_t ‘*out’, size_t ‘ndim’) For every dimension, add the coordinates in ‘c1’ with ‘c2’ and put the result into ‘out’. In other words, for dimension ‘i’ run ‘out[i]=c1[i]+c2[i];’. Hence ‘out’ may be equal to any one of ‘c1’ or ‘c2’. -- Function: size_t gal_dimension_coord_to_index (size_t ‘ndim’, size_t ‘*dsize’, size_t ‘*coord’) Return the index (counting from zero) from the coordinates in ‘coord’ (counting from zero) assuming the dataset has ‘ndim’ elements and the size of the dataset along each dimension is in the ‘dsize’ array. -- Function: void gal_dimension_index_to_coord (size_t ‘index’, size_t ‘ndim’, size_t ‘*dsize’, size_t ‘*coord’) Fill in the ‘coord’ array with the coordinates that correspond to ‘index’ assuming the dataset has ‘ndim’ elements and the size of the dataset along each dimension is in the ‘dsize’ array. Note that both ‘index’ and each value in ‘coord’ are assumed to start from ‘0’ (zero). Also that the space which ‘coord’ points to must already be allocated before calling this function. -- Function: size_t gal_dimension_dist_manhattan (size_t ‘*a’, size_t ‘*b’, size_t ‘ndim’) Return the manhattan distance (see Wikipedia (https://en.wikipedia.org/wiki/Taxicab_geometry)) between the two coordinates ‘a’ and ‘b’ (each an array of ‘ndim’ elements). -- Function-like macro: GAL_DIMENSION_NEIGHBOR_OP (‘index’, ‘ndim’, ‘dsize’, ‘connectivity’, ‘dinc’, ‘operation’) Parse the neighbors of the element located at ‘index’ and do the requested operation on them. This is defined as a macro to allow easy definition of any operation on the neighbors of a given element without having to use loops within your source code (the loops are implemented by this macro). For an example of using this function, please see *note Library demo - inspecting neighbors::. The input arguments to this function-like macro are described below: ‘index’ Distance of this element from the first element in the array on a contiguous patch of memory (starting from 0), see the discussion above. ‘ndim’ The number of dimensions associated with the contiguous patch of memory. ‘dsize’ The full array size along each dimension. This must be an array and is assumed to have the same number elements as ‘ndim’. See the discussion under the same element in *note Generic data container::. ‘connectivity’ Most distant neighbors to consider. Depending on the number of dimensions, different neighbors may be defined for each element. This function-like macro distinguish between these different neighbors with this argument. It has a value between ‘1’ (one) and ‘ndim’. For example in a 2D dataset, 4-connected neighbors have a connectivity of ‘1’ and 8-connected neighbors have a connectivity of ‘2’. Note that this is inclusive, so in this example, a connectivity of ‘2’ will also include connectivity ‘1’ neighbors. ‘dinc’ An array keeping the length necessary to increment along each dimension. You can make this array with the following function. Just don’t forget to free the array after you are done with it: size_t *dinc=gal_dimension_increment(ndim, dsize); ‘dinc’ depends on ‘ndim’ and ‘dsize’, but it must be defined outside this function-like macro since it involves allocation to help in performance. ‘operation’ Any C operation that you would like to do on the neighbor. This macro will provide you a ‘nind’ variable that can be used as the index of the neighbor that is currently being studied. It is defined as ‘‘size_t ndim;’’. Note that ‘operation’ will be repeated the number of times there is a neighbor for this element. This macro works fully within its own ‘{}’ block and except for the ‘nind’ variable that shows the neighbor’s index, all the variables within this macro’s block start with ‘gdn_’.  File: gnuastro.info, Node: Linked lists, Next: FITS files, Prev: Dimensions, Up: Gnuastro library 10.3.7 Linked lists (‘list.h’) ------------------------------ An array is a contiguous region of memory that is very efficient and easy to use for recording and later accessing any random element as fast as any other. This makes array the primary data container when you have many elements (for example an image which has millions of pixels). One major problem with an array is that the number of elements that go into it must be known in advance and adding or removing an element will require a re-set of all the other elements. For example if you want to remove the 3rd element in a 1000 element array, all 997 subsequent elements have to pulled back by one position, the reverse will happen if you need to add an element. In many contexts such situations never come up, for example you don’t want to shift all the pixels in an image by one or two pixels from some random position in the image: their positions have scientific value. But in other contexts you will find your self frequently adding/removing an a-priori unknown number of elements. Linked lists (or _lists_ for short) are the data-container of choice in such situations. As in a chain, each _node_ in a list is an independent C structure, keeping its own data along with pointer(s) to its immediate neighbor(s). Below, you can see one simple linked list node structure along with an ASCII art schematic of how we can use the ‘next’ pointer to add any number of elements to the list that we want. By convention, a list is terminated when ‘next’ is the ‘NULL’ pointer. struct list_float /* --------- --------- */ { /* | Value | | Value | */ float value; /* | --- | | --- | */ struct list_float *next; /* | next-|--> | next-|--> NULL */ } /* --------- --------- */ The schematic shows another great advantage of linked lists: it is very easy to add or remove/pop a node anywhere in the list. If you want to modify the first node, you just have to change one pointer. If it is in the middle, you just have to change two. You initially define a variable of this type with a ‘NULL’ pointer as shown below: struct list_float *mylist=NULL; To add or remove/pop a node from the list you can use functions provided for the respective type in the sections below. When you add an element to the list, it is conventionally added to the “top†of the list: the general list pointer will point to the newly created node, which will point to the previously created node and so on. So when you “pop†from the top of the list, you are actually retrieving the last value you put in and changing the list pointer to the next youngest node. This is thus known as a “last-in-first-out†list. This is the most efficient type of linked list (easier to implement and faster to process). Alternatively, you can add each newly created node at the end of the list. If you do that, you will get a “first-in-first-out†list. But that will force you to go through the whole list for each new element that is created (this will slow down the processing)(1). The node example above creates the simplest kind of a list. We can define each node with two pointers to both the next and previous neighbors, this is called a “Doubly linked listâ€. In general, lists are very powerful and simple constructs that can be very useful. But going into more detail would be out of the scope of this short introduction in this book. Wikipedia (https://en.wikipedia.org/wiki/Linked_list) has a nice and more thorough discussion of the various types of lists. To appreciate/use the beauty and elegance of these powerful constructs even further, see Chapter 2 (Information Structures, in volume 1) of Donald Knuth’s “The art of computer programmingâ€. In this section we will review the functions and structures that are available in Gnuastro for working on lists. They differ by the type of data that each node can keep. For each linked-list node structure, we will first introduce the structure, then the functions for working on the structure. All these structures and functions are defined and declared in ‘gnuastro/list.h’. * Menu: * List of strings:: Simply linked list of strings. * List of int32_t:: Simply linked list of int32_ts. * List of size_t:: Simply linked list of size_ts. * List of float:: Simply linked list of floats. * List of double:: Simply linked list of doubles * List of void:: Simply linked list of void * pointers. * Ordered list of size_t:: Simply linked, ordered list of size_t. * Doubly linked ordered list of size_t:: Definition and functions. * List of gal_data_t:: Simply linked list Gnuastro’s generic datatype. ---------- Footnotes ---------- (1) A better way to get a first-in-first-out is to first keep the data as last-in-first-out until they are all read. Afterwards, reverse the list by popping each node and immediately add it to the new list. This practically reverses the last-in-first-out list to a first-in-first-out one. All the list types discussed in this chapter have a function with a ‘_reverse’ suffix for this job.  File: gnuastro.info, Node: List of strings, Next: List of int32_t, Prev: Linked lists, Up: Linked lists 10.3.7.1 List of strings ........................ Probably one of the most common lists you will be using are lists of strings. They are the best tools when you are reading the user’s inputs, or when adding comments to the output files. Below you can see Gnuastro’s string list type and several functions to help in adding, removing/popping, reversing and freeing the list. -- Type (C ‘struct’): gal_list_str_t A single node in a list containing a string of characters. typedef struct gal_list_str_t { char *v; struct gal_list_str_t *next; } gal_list_str_t; -- Function: void gal_list_str_add (gal_list_str_t ‘**list’, char ‘*value’, int ‘allocate’) Add a new node to the list of strings (‘list’) and update it. The new node will contain the string ‘value’. If ‘allocate’ is not zero, space will be allocated specifically for the string of the new node and the contents of ‘value’ will be copied into it. This can be useful when your string may be changed later in the program, but you want your list to remain. Here is one short/simple example of initializing and adding elements to a string list: gal_list_str_t *strlist; gal_list_str_add(&strlist, "bottom of list."); gal_list_str_add(&strlist, "second last element of list."); -- Function: char * gal_list_str_pop (gal_list_str_t ‘**list’) Pop the top element of ‘list’, change ‘list’ to point to the next node in the list, and return the string that was in the popped node. If ‘*list==NULL’, then this function will also return a ‘NULL’ pointer. -- Function: size_t gal_list_str_number (gal_list_str_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_str_print (gal_list_str_t ‘*list’) Print the strings within each node of ‘*list’ on the standard output in the same order that they are stored. Each string is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly, format. For example the following code snippet. size_t i; gal_list_str_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("String %zu: %s\n", i, tmp->v); -- Function: void gal_list_str_reverse (gal_list_str_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: void gal_list_str_free (gal_list_str_t ‘*list’, int ‘freevalue’) Free every node in ‘list’. If ‘freevalue’ is not zero, also free the string within the nodes.  File: gnuastro.info, Node: List of int32_t, Next: List of size_t, Prev: List of strings, Up: Linked lists 10.3.7.2 List of ‘int32_t’ .......................... Signed integers are the best types when you are dealing with a positive or negative integers. The are generally useful in many contexts, for example when you want to keep the order of a series of states (each state stored as a given number in an ‘enum’ for example). On many modern systems, ‘int32_t’ is just an alias for ‘int’, so you can use them interchangeably. To make sure, check the size of ‘int’ on your system: -- Type (C ‘struct’): gal_list_i32_t A single node in a list containing a 32-bit signed integer (see *note Numeric data types::). typedef struct gal_list_i32_t { int32_t v; struct gal_list_i32_t *next; } gal_list_i32_t; -- Function: void gal_list_i32_add (gal_list_i32_t ‘**list’, int32_t ‘value’) Add a new node (containing ‘value’) to the top of the ‘list’ of ‘int32_t’s (‘uint32_t’ is equal to ‘int’ on many modern systems), and update ‘list’. Here is one short example of initializing and adding elements to a string list: gal_list_i32_t *i32list=NULL; gal_list_i32_add(&i32list, 52); gal_list_i32_add(&i32list, -4); -- Function: int32_t gal_list_i32_pop (gal_list_i32_t ‘**list’) Pop the top element of ‘list’ and return the value. This function will also change ‘list’ to point to the next node in the list. If ‘*list==NULL’, then this function will also return ‘GAL_BLANK_INT32’ (see *note Library blank values::). -- Function: size_t gal_list_i32_number (gal_list_i32_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_i32_print (gal_list_i32_t ‘*list’) Print the integers within each node of ‘*list’ on the standard output in the same order that they are stored. Each integer is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. size_t i; gal_list_i32_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("String %zu: %s\n", i, tmp->v); -- Function: void gal_list_i32_reverse (gal_list_i32_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: int32_t * gal_list_i32_to_array (gal_list_i32_t ‘*list’, int ‘reverse’, size_t ‘*num’) Dynamically allocate an array and fill it with the values in ‘list’. The function will return a pointer to the allocated array and put the number of elements in the array into the ‘num’ pointer. If ‘reverse’ has a non-zero value, the array will be filled in the opposite order of elements in ‘list’. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. -- Function: void gal_list_i32_free (gal_list_i32_t ‘*list’) Free every node in ‘list’.  File: gnuastro.info, Node: List of size_t, Next: List of float, Prev: List of int32_t, Up: Linked lists 10.3.7.3 List of ‘size_t’ ......................... The ‘size_t’ type is a unique type in C: as the name suggests it is defined to store sizes, or more accurately, the distances between memory locations. Hence it is always positive (an ‘unsigned’ type) and it is directly related to the address-able spaces on the host system: on 32-bit and 64-bit systems it is an alias for ‘uint32_t’ and ‘uint64_t’, respectively (see *note Numeric data types::). ‘size_t’ is the default compiler type to index an array (recall that an array index in C is just a pointer increment of a given _size_). Since it is unsigned, its a great type for counting (where negative is not defined), you are always sure it will never exceed the system’s (virtual) memory and since its name has the word “size†inside it, it provides a good level of documentation(1). In Gnuastro, we do all counting and array indexing with this type, so this list is very handy. As discussed above, ‘size_t’ maps to different types on different machines, so a portable way to print them with ‘printf’ is to use C99’s ‘%zu’ format. -- Type (C ‘struct’): gal_list_sizet_t A single node in a list containing a ‘size_t’ value (which maps to ‘uint32_t’ or ‘uint64_t’ on 32-bit and 64-bit systems), see *note Numeric data types::. typedef struct gal_list_sizet_t { size_t v; struct gal_list_sizet_t *next; } gal_list_sizet_t; -- Function: void gal_list_sizet_add (gal_list_sizet_t ‘**list’, size_t ‘value’) Add a new node (containing ‘value’) to the top of the ‘list’ of ‘size_t’s and update ‘list’. Here is one short example of initializing and adding elements to a string list: gal_list_sizet_t *slist=NULL; gal_list_sizet_add(&slist, 45493); gal_list_sizet_add(&slist, 930484); -- Function: sizet_t gal_list_sizet_pop (gal_list_sizet_t ‘**list’) Pop the top element of ‘list’ and return the value. This function will also change ‘list’ to point to the next node in the list. If ‘*list==NULL’, then this function will also return ‘GAL_BLANK_SIZE_T’ (see *note Library blank values::). -- Function: size_t gal_list_sizet_number (gal_list_sizet_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_sizet_print (gal_list_sizet_t ‘*list’) Print the values within each node of ‘*list’ on the standard output in the same order that they are stored. Each integer is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example, the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. size_t i; gal_list_sizet_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("String %zu: %zu\n", i, tmp->v); -- Function: void gal_list_sizet_reverse (gal_list_sizet_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: size_t * gal_list_sizet_to_array (gal_list_sizet_t ‘*list’, int ‘reverse’, size_t ‘*num’) Dynamically allocate an array and fill it with the values in ‘list’. The function will return a pointer to the allocated array and put the number of elements in the array into the ‘num’ pointer. If ‘reverse’ has a non-zero value, the array will be filled in the inverse of the order of elements in ‘list’. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. -- Function: void gal_list_sizet_free (gal_list_sizet_t ‘*list’) Free every node in ‘list’. ---------- Footnotes ---------- (1) So you know that a variable of this type is not used to store some generic state for example.  File: gnuastro.info, Node: List of float, Next: List of double, Prev: List of size_t, Up: Linked lists 10.3.7.4 List of ‘float’ ........................ Single precision floating point numbers can accurately store real number until 7.2 decimals and only consume 4 bytes (32-bits) of memory, see *note Numeric data types::. Since astronomical data rarely reach that level of precision, single precision floating points are the type of choice to keep and read data. However, when processing the data, it is best to use double precision floating points (since errors propagate). -- Type (C ‘struct’): gal_list_f32_t A single node in a list containing a 32-bit single precision ‘float’ value: see *note Numeric data types::. typedef struct gal_list_f32_t { float v; struct gal_list_f32_t *next; } gal_list_f32_t; -- Function: void gal_list_f32_add (gal_list_f32_t ‘**list’, float ‘value’) Add a new node (containing ‘value’) to the top of the ‘list’ of ‘float’s and update ‘list’. Here is one short example of initializing and adding elements to a string list: gal_list_f32_t *flist=NULL; gal_list_f32_add(&flist, 3.89); gal_list_f32_add(&flist, 1.23e-20); -- Function: float gal_list_f32_pop (gal_list_f32_t ‘**list’) Pop the top element of ‘list’ and return the value. This function will also change ‘list’ to point to the next node in the list. If ‘*list==NULL’, then this function will return ‘GAL_BLANK_FLOAT32’ (NaN, see *note Library blank values::). -- Function: size_t gal_list_f32_number (gal_list_f32_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_f32_print (gal_list_f32_t ‘*list’) Print the values within each node of ‘*list’ on the standard output in the same order that they are stored. Each floating point number is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example, in the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. size_t i; gal_list_f32_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("Node %zu: %f\n", i, tmp->v); -- Function: void gal_list_f32_reverse (gal_list_f32_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: float * gal_list_f32_to_array (gal_list_f32_t ‘*list’, int ‘reverse’, size_t ‘*num’) Dynamically allocate an array and fill it with the values in ‘list’. The function will return a pointer to the allocated array and put the number of elements in the array into the ‘num’ pointer. If ‘reverse’ has a non-zero value, the array will be filled in the inverse of the order of elements in ‘list’. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. -- Function: void gal_list_f32_free (gal_list_f32_t ‘*list’) Free every node in ‘list’.  File: gnuastro.info, Node: List of double, Next: List of void, Prev: List of float, Up: Linked lists 10.3.7.5 List of ‘double’ ......................... Double precision floating point numbers can accurately store real number until 15.9 decimals and consume 8 bytes (64-bits) of memory, see *note Numeric data types::. This level of precision makes them very good for serious processing in the middle of a program’s execution: in many cases, the propagation of errors will still be insignificant compared to actual observational errors in a data set. But since they consume 8 bytes and more CPU processing power, they are often not the best choice for storing and transferring of data. -- Type (C ‘struct’): gal_list_f64_t A single node in a list containing a 64-bit double precision ‘double’ value: see *note Numeric data types::. typedef struct gal_list_f64_t { double v; struct gal_list_f64_t *next; } gal_list_f64_t; -- Function: void gal_list_f64_add (gal_list_f64_t ‘**list’, double ‘value’) Add a new node (containing ‘value’) to the top of the ‘list’ of ‘double’s and update ‘list’. Here is one short example of initializing and adding elements to a string list: gal_list_f64_t *dlist=NULL; gal_list_f64_add(&dlist, 3.8129395763193); gal_list_f64_add(&dlist, 1.239378923931e-20); -- Function: double gal_list_f64_pop (gal_list_f64_t ‘**list’) Pop the top element of ‘list’ and return the value. This function will also change ‘list’ to point to the next node in the list. If ‘*list==NULL’, then this function will return ‘GAL_BLANK_FLOAT64’ (NaN, see *note Library blank values::). -- Function: size_t gal_list_f64_number (gal_list_f64_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_f64_print (gal_list_f64_t ‘*list’) Print the values within each node of ‘*list’ on the standard output in the same order that they are stored. Each floating point number is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example, in the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. size_t i; gal_list_f64_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("Node %zu: %f\n", i, tmp->v); -- Function: void gal_list_f64_reverse (gal_list_f64_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: double * gal_list_f64_to_array (gal_list_f64_t ‘*list’, int ‘reverse’, size_t ‘*num’) Dynamically allocate an array and fill it with the values in ‘list’. The function will return a pointer to the allocated array and put the number of elements in the array into the ‘num’ pointer. If ‘reverse’ has a non-zero value, the array will be filled in the inverse of the order of elements in ‘list’. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. -- Function: void gal_list_f64_free (gal_list_f64_t ‘*list’) Free every node in ‘list’.  File: gnuastro.info, Node: List of void, Next: Ordered list of size_t, Prev: List of double, Up: Linked lists 10.3.7.6 List of ‘void *’ ......................... In C, ‘void *’ is the most generic pointer. Usually pointers are associated with the type of content they point to. For example ‘int *’ means a pointer to an integer. This ancillary information about the contents of the memory location is very useful for the compiler, catching bad errors and also documentation (it helps the reader see what the address in memory actually contains). However, ‘void *’ is just a raw address (pointer), it contains no information on the contents it points to. These properties make the ‘void *’ very useful when you want to treat the contents of an address in different ways. You can use the ‘void *’ list defined in this section and its function on any kind of data: for example you can use it to keep a list of custom data structures that you have built for your own separate program. Each node in the list can keep anything and this gives you great versatility. But in using ‘void *’, please beware that “with great power comes great responsibilityâ€. -- Type (C ‘struct’): gal_list_void_t A single node in a list containing a ‘void *’ pointer. typedef struct gal_list_void_t { void *v; struct gal_list_void_t *next; } gal_list_void_t; -- Function: void gal_list_void_add (gal_list_void_t ‘**list’, void ‘*value’) Add a new node (containing ‘value’) to the top of the ‘list’ of ‘void *’s and update ‘list’. Here is one short example of initializing and adding elements to a string list: gal_list_void_t *vlist=NULL; gal_list_f64_add(&vlist, some_pointer); gal_list_f64_add(&vlist, another_pointer); -- Function: void * gal_list_void_pop (gal_list_void_t ‘**list’) Pop the top element of ‘list’ and return the value. This function will also change ‘list’ to point to the next node in the list. If ‘*list==NULL’, then this function will return ‘NULL’. -- Function: size_t gal_list_void_number (gal_list_void_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_void_reverse (gal_list_void_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: void gal_list_void_free (gal_list_void_t ‘*list’) Free every node in ‘list’.  File: gnuastro.info, Node: Ordered list of size_t, Next: Doubly linked ordered list of size_t, Prev: List of void, Up: Linked lists 10.3.7.7 Ordered list of ‘size_t’ ................................. Positions/sizes in a dataset are conventionally in the ‘size_t’ type (see *note List of size_t::) and it sometimes occurs that you want to parse and read the values in a specific order. For example you want to start from one pixel and add pixels to the list based on their distance to that pixel. So that ever time you pop an element from the list, you know it is the nearest that has not yet been studied. The ‘gal_list_osizet_t’ type and its functions in this section are designed to facilitate such operations. -- Type (C ‘struct’): gal_list_osizet_t Each node in this singly-linked list contains a ‘size_t’ value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. At any moment, the first popped node in this list will have the smallest ‘tosort’ value, and subsequent nodes will have larger to values. typedef struct gal_list_osizet_t { size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_list_osizet_t *next; } gal_list_osizet_t; -- Function: void gal_list_osizet_add (gal_list_osizet_t ‘**list’, size_t ‘value’, float ‘tosort’) Allocate space for a new node in ‘list’, and store ‘value’ and ‘tosort’ into it. The new node will not necessarily be at the “top†of the list. If ‘*list!=NULL’, then the ‘tosort’ values of existing nodes is inspected and the given node is placed in the list such that the top element (which is popped with ‘gal_list_osizet_pop’) has the smallest ‘tosort’ value. -- Function: size_t gal_list_osizet_pop (gal_list_osizet_t ‘**list’, float ‘*sortvalue’) Pop a node from the top of ‘list’, return the node’s ‘value’ and put its sort value in the space that ‘sortvalue’ points to. This function will also free the allocated space for the popped node and after this function, ‘list’ will point to the next node (which has a larger ‘tosort’ element). -- Function: void gal_list_osizet_to_sizet_free (gal_list_osizet_t ‘*in’, gal_list_sizet_t ‘**out’) Convert the ordered list of ‘size_t’s into an ordinary ‘size_t’ linked list. This can be useful when all the elements have been added and you just need to pop-out elements and don’t care about the sorting values any more. After the conversion is done, this function will free the input list. Note that the ‘out’ list doesn’t have to be empty. If it already contains some nodes, the new nodes will be added on top of them.  File: gnuastro.info, Node: Doubly linked ordered list of size_t, Next: List of gal_data_t, Prev: Ordered list of size_t, Up: Linked lists 10.3.7.8 Doubly linked ordered list of ‘size_t’ ............................................... An ordered list of indexs is required in many contexts, one example was discussed at the beginning of *note Ordered list of size_t::. But the list that was introduced there only has one point of entry: you can always only parse the list from smallest to largest. In this section, the doubly-linked ‘gal_list_dosizet_t’ node is defined which will allow us to parse the values in ascending or descending order. -- Type (C ‘struct’): gal_list_dosizet_t Doubly-linked, ordered ‘size_t’ list node structure. Each node in this Doubly-linked list contains a ‘size_t’ value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. In the functions here, this linked list can be pointed to by two pointers (largest and smallest) with the following format: largest pointer | NULL <-- (v0,s0) <--> (v1,s1) <--> ... (vn,sn) --> NULL | smallest pointer At any moment, the two pointers will point to the nodes containing the “largest†and “smallest†values and the rest of the nodes will be sorted. This is useful when an unknown number of nodes are being added continuously and during the operations it is important to have the nodes in a sorted format. typedef struct gal_list_dosizet_t { size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_list_dosizet_t *prev; struct gal_list_dosizet_t *next; } gal_list_dosizet_t; -- Function: void gal_list_dosizet_add (gal_list_dosizet_t ‘**largest’, gal_list_dosizet_t ‘**smallest’, size_t ‘value’, float ‘tosort’) Allocate space for a new node in ‘list’, and store ‘value’ and ‘tosort’ into it. If the list is empty, both ‘largest’ and ‘smallest’ must be ‘NULL’. -- Function: size_t gal_list_dosizet_pop_smallest (gal_list_dosizet_t ‘**largest’, gal_list_dosizet_t ‘**smallest’, float ‘tosort’) Pop the value with the smallest reference from the doubly linked list and store the reference into the space pointed to by ‘tosort’. Note that even though only the smallest pointer will be popped, when there was only one node in the list, the ‘largest’ pointer also has to change, so we need both. -- Function: void gal_list_dosizet_print (gal_list_dosizet_t ‘*largest’, gal_list_dosizet_t ‘*smallest’) Print the largest and smallest values sequentially until the list is parsed. -- Function: void gal_list_dosizet_to_sizet (gal_list_dosizet_t ‘*in’, gal_list_sizet_t ‘**out’) Convert the doubly linked, ordered ‘size_t’ list into a singly-linked list of ‘size_t’. -- Function: void gal_list_dosizet_free (gal_list_dosizet_t ‘*largest’) Free the doubly linked, ordered ‘sizet_t’ list.  File: gnuastro.info, Node: List of gal_data_t, Prev: Doubly linked ordered list of size_t, Up: Linked lists 10.3.7.9 List of ‘gal_data_t’ ............................. Gnuastro’s generic data container has a ‘next’ element which enables it to be used as a singly-linked list (see *note Generic data container::). The ability to connect the different data containers offers great advantages. For example each column in a table in an independent dataset: with its own name, units, numeric data type (see *note Numeric data types::). Another application is in Tessellating an input dataset into separate tiles or only studying particular regions, or tiles, of a larger dataset (see *note Tessellation:: and *note Tessellation library::). Each independent tile over the dataset can be connected to the others as a linked list and thus any number of tiles can be represented with one variable. -- Function: void gal_list_data_add (gal_data_t ‘**list’, gal_data_t ‘*newnode’) Add an already allocated dataset (‘newnode’) to top of ‘list’. Note that if ‘newnode->next!=NULL’ (‘newnode’ is itself a list), then ‘list’ will be added to its end. In this example multiple images are linked together as a list: size_t minmapsize=-1; gal_data_t *tmp, *list=NULL; tmp = gal_fits_img_read("file1.fits", "1", minmapsize, 0, 0); gal_list_data_add( &list, tmp ); tmp = gal_fits_img_read("file2.fits", "1", minmapsize, 0, 0); gal_list_data_add( &list, tmp ); -- Function: void gal_list_data_add_alloc (gal_data_t ‘**list’, void ‘*array’, uint8_t ‘type’, size_t ‘ndim’, size_t ‘*dsize’, struct wcsprm ‘*wcs’, int ‘clear’, size_t ‘minmapsize’, char ‘*name’, char ‘*unit’, char ‘*comment’) Allocate a new dataset (with ‘gal_data_alloc’ in *note Dataset size and allocation::) and put it as the first element of ‘list’. Note that if this is the first node to be added to the list, ‘list’ must be ‘NULL’. -- Function: gal_data_t * gal_list_data_pop (gal_data_t ‘**list’) Pop the top node from ‘list’ and return it. -- Function: void gal_list_data_reverse (gal_data_t ‘**list’) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. -- Function: size_t gal_list_data_number (gal_data_t ‘*list’) Return the number of nodes in ‘list’. -- Function: void gal_list_data_free (gal_data_t ‘*list’) Free all the datasets in ‘list’ along with all the allocated spaces in each.  File: gnuastro.info, Node: FITS files, Next: World Coordinate System, Prev: Linked lists, Up: Gnuastro library 10.3.8 FITS files (‘fits.h’) ---------------------------- The FITS format is the most common format to store data (images and tables) in astronomy. The CFITSIO library already provides a very good low-level collection of functions for manipulating FITS data. The low-level nature of CFITSIO is defined for versatility and portability. As a result, even a simple a basic operation, like reading an image or table column into memory, will require a special sequence of CFITSIO function calls which can be inconvenient and buggy to manage in separate locations. Therefore Gnuastro library provides wrappers for CFITSIO functions to make it much easier to read/write/modify FITS file data, header keywords and extensions. Hence, if you feel these functions don’t exactly do what you want, we strongly recommend reading the CFITSIO manual to use its great features directly. All the functions and macros introduced in this section are declared in ‘gnuastro/fits.h’. When you include this header, you are also including CFITSIO’s ‘fitsio.h’ header. So you don’t need to explicitly include ‘fitsio.h’ anymore and can freely use any of its macros or functions in your code along with those discussed here. * Menu: * FITS macros errors filenames:: General macros, errors and checking names. * CFITSIO and Gnuastro types:: Conversion between FITS and Gnuastro types. * FITS HDUs:: Opening and getting information about HDUs. * FITS header keywords:: Reading and writing FITS header keywords. * FITS arrays:: Reading and writing FITS images/arrays. * FITS tables:: Reading and writing FITS tables.  File: gnuastro.info, Node: FITS macros errors filenames, Next: CFITSIO and Gnuastro types, Prev: FITS files, Up: FITS files 10.3.8.1 FITS Macros, errors and filenames .......................................... Some general constructs provided by Gnuastro’s FITS handling functions are discussed here. In particular there are several useful functions about FITS file names. -- Macro: GAL_FITS_MAX_NDIM The maximum number of dimensions a dataset can have in FITS format, according to the FITS standard this is 999. -- Function: void gal_fits_io_error (int ‘status’, char ‘*message’) If ‘status’ is non-zero, this function will print the CFITSIO error message corresponding to status, print ‘message’ (optional) in the next line and abort the program. If ‘message==NULL’, it will print a default string after the CFITSIO error. -- Function: int gal_fits_name_is_fits (char ‘*name’) If the ‘name’ is an acceptable CFITSIO FITS filename return ‘1’ (one), otherwise return ‘0’ (zero). The currently acceptable FITS suffixes are ‘.fits’, ‘.fit’, ‘.fits.gz’, ‘.fits.Z’, ‘.imh’, ‘.fits.fz’. IMH is the IRAF format which is acceptable to CFITSIO. -- Function: int gal_fits_suffix_is_fits (char ‘*suffix’) Similar to ‘gal_fits_name_is_fits’, but only for the suffix. The suffix doesn’t have to start with ‘<.>’: this function will return ‘1’ (one) for both ‘fits’ and ‘.fits’. -- Function: char * gal_fits_name_save_as_string (char ‘*filename’, char ‘*hdu’) If the name is a FITS name, then put a ‘(hdu: ...)’ after it and return the string. If it isn’t a FITS file, just print the name. Note that the space is allocated. This function is useful when you want to report a random file to the user which may be FITS or not (for a FITS file, simply the filename is not enough, the HDU is also necessary).  File: gnuastro.info, Node: CFITSIO and Gnuastro types, Next: FITS HDUs, Prev: FITS macros errors filenames, Up: FITS files 10.3.8.2 CFITSIO and Gnuastro types ................................... Both Gnuastro and CFITSIO have special identifiers for each type that they accept. Gnuastro’s type identifiers are fully described in *note Library data types:: and are usable for all kinds of datasets (images, table columns and etc) as part of Gnuastro’s *note Generic data container::. However, following the FITS standard, CFITSIO has different identifiers for images and tables. Following CFITSIO’s own convention, we will use ‘bitpix’ for image type identifiers and ‘datatype’ for its internal identifiers (and mainly used in tables). The functions introduced in this section can be used to convert between CFITSIO and Gnuastro’s type identifiers. One important issue to consider is that CFITSIO’s types are not fixed width (for example ‘long’ may be 32-bits or 64-bits on different systems). However, Gnuastro’s types are defined by their width. These functions will use information on the host system to do the proper conversion, so it strongly recommended to use these functions for portability of your code and not to assume a fixed correspondence between CFITSIO and Gnuastro’s types. -- Function: uint8_t gal_fits_bitpix_to_type (int ‘bitpix’) Return the Gnuastro type identifier that corresponds to CFITSIO’s ‘bitpix’ on this system. -- Function: int gal_fits_type_to_bitpix (uint8_t ‘type’) Return the CFITSIO ‘bitpix’ value that corresponds to Gnuastro’s ‘type’. -- Function: char gal_fits_type_to_bin_tform (uint8_t ‘type’) Return the FITS standard binary table ‘TFORM’ character that corresponds to Gnuastro’s ‘type’. -- Function: int gal_fits_type_to_datatype (uint8_t ‘type’) Return the CFITSIO ‘datatype’ that corresponds to Gnuastro’s ‘type’ on this machine. -- Function: uint8_t gal_fits_datatype_to_type (int ‘datatype’, int ‘is_table_column’) Return Gnuastro’s type identifier that corresponds to the CFITSIO ‘datatype’. Note that when dealing with CFITSIO’s ‘TLONG’, the fixed width type differs between tables and images. So if the corresponding dataset is a table column, put a non-zero value into ‘is_table_column’.  File: gnuastro.info, Node: FITS HDUs, Next: FITS header keywords, Prev: CFITSIO and Gnuastro types, Up: FITS files 10.3.8.3 FITS HDUs .................. A FITS file can contain multiple HDUs/extensions. The functions in this section can be used to get basic information about the extensions or open them. Note that ‘fitsfile’ is defined in CFITSIO’s ‘fitsio.h’ which is automatically included by Gnuastro’s ‘gnuastro/fits.h’. -- Function: fitsfile * gal_fits_open_to_write (char ‘*filename’) If ‘filename’ exists, open it and return the ‘fitsfile’ pointer that corresponds to it. If ‘filename’ doesn’t exist, the file will be created which contains a blank first extension and the pointer to its next extension will be returned. -- Function: size_t gal_fits_hdu_num (char ‘*filename’) Return the number of HDUs/extensions in ‘filename’. -- Function: int gal_fits_hdu_format (char ‘*filename’, char ‘*hdu’) Return the format of the HDU as one of CFITSIO’s recognized macros: ‘IMAGE_HDU’, ‘ASCII_TBL’, or ‘BINARY_TBL’. -- Function: fitsfile * gal_fits_hdu_open (char ‘*filename’, char ‘*hdu’, int ‘iomode’) Open the HDU/extension ‘hdu’ from ‘filename’ and return a pointer to CFITSIO’s ‘fitsfile’. ‘iomode’ determines how the FITS file will be opened using CFITSIO’s macros: ‘READONLY’ or ‘READWRITE’. The string in ‘hdu’ will be appended to ‘filename’ in square brackets so CFITSIO only opens this extension. You can use any formatting for the ‘hdu’ that is acceptable to CFITSIO. See the description under ‘--hdu’ in *note Input output options:: for more. -- Function: fitsfile * gal_fits_hdu_open_format (char ‘*filename’, char ‘*hdu’, int ‘img0_tab1’) Open (in read-only format) the ‘hdu’ HDU/extension of ‘filename’ as an image or table. When ‘img0_tab1’ is ‘0’(zero) but the HDU is a table, this function will abort with an error. It will also abort with an error when ‘img0_tab1’ is ‘1’ (one), but the HDU is an image. A FITS HDU may contain both tables or images. When your program needs one of these formats, you can call this function so if the user provided the wrong HDU/file, it will abort and inform the user that the file/HDU is has the wrong format.  File: gnuastro.info, Node: FITS header keywords, Next: FITS arrays, Prev: FITS HDUs, Up: FITS files 10.3.8.4 FITS header keywords ............................. Each FITS extension/HDU contains a raw dataset which can either be a table or an image along with some header keywords. The keywords can be used to store meta-data about the actual dataset. The functions in this section describe Gnuastro’s high-level functions for reading and writing FITS keywords. Similar to all Gnuastro’s FITS-related functions, these functions are all wrappers for CFITSIO’s low-level functions. The necessary meta-data (header keywords) for a particular dataset are commonly numerous, it is much more efficient to list them in one variable and call the reading/writing functions once. Hence the functions in this section use linked lists, a thorough introduction to them is given in *note Linked lists::. To reading FITS keywords, these functions use a list of Gnuastro’s generic dataset format that is discussed in *note List of gal_data_t::. To write FITS keywords we define the ‘gal_fits_list_key_t’ node that is defined below. -- Type (C ‘struct’): gal_fits_list_key_t Structure for writing FITS keywords. This structure is used for one keyword and you don’t need to set all elements. With the ‘next’ element, you can link it to another keyword thus creating a linked list to add any number of keywords easily and at any step during your program (see *note Linked lists:: for an introduction on lists). See the functions below for adding elements to the list. typedef struct gal_fits_list_key_t { int kfree; /* ==1, free name. */ int vfree; /* ==1, free value. */ int cfree; /* ==1, free comment. */ uint8_t type; /* Keyword value type. */ char *keyname; /* Keyword Name. */ void *value; /* Keyword value. */ char *comment; /* Keyword comment. */ char *unit; /* Keyword unit. */ struct gal_fits_list_key_t *next; /* Next keyword. */ } gal_fits_list_key_t; -- Function: void * gal_fits_key_img_blank (uint8_t ‘type’) Returns a pointer to an allocated space for the FITS ‘BLANK’ header keyword when the input array has a type of ‘type’. According to the FITS standard: “If the ‘BSCALE’ and ‘BZERO’ keywords do not have the default values of 1.0 and 0.0, respectively, then the value of the ‘BLANK’ keyword must equal the actual value in the FITS data array that is used to represent an undefined pixel and not the corresponding physical valueâ€. Therefore a special ‘BLANK’ value is needed for datasets containing signed 8-bit integers and unsigned 16-bit, 32-bit and 64-bit integers (types that are defined with ‘BSCALE’ and ‘BZERO’ in the FITS standard). -- Function: void gal_fits_key_clean_str_value (char ‘*string’) Remove the single quotes and possible extra spaces around the keyword values that CFITSIO returns when reading a string keyword. CFITSIO doesn’t remove the two single quotes around the string value of a keyword. Hence the strings it reads are like: ‘'value '’, or ‘'some_very_long_value'’. To use the value during your processing, it is commonly necessary to remove the single quotes (and possible extra spaces). This function will do this within the allocated space of the string. -- Function: void gal_fits_key_read_from_ptr (fitsfile ‘*fptr’, gal_data_t ‘*keysll’, int ‘readcomment’, int ‘readunit’) Read the list of keyword values from a FITS pointer. The input should be a linked list of Gnuastro’s generic data container (‘gal_data_t’). Before calling this function, you just have to set the ‘name’ and desired ‘type’ values of each node in the list to the keyword you want it to keep the value of. The given ‘name’ value will be directly passed to CFITSIO to read the desired keyword name. This function will allocate space to keep the value. If ‘readcomment’ and ‘readunit’ are non-zero, this function will also try to read the possible comments and units of the keyword. Here is one example of using this function: /* Allocate an array of datasets. */ gal_data_t *keysll=gal_data_array_calloc(N); /* Use the array as a list.*/ for(i=0;i0) and used as the keyword name. The FITS standard sets a maximum length for the value of a keyword. This creates problems with file names (which include directories). Because file names/addresses can become very long. Therefore, when ‘filename’ is longer than the maximum length of a FITS keyword value, this function will break it into several keywords (breaking up the string on directory separators). -- Function: void gal_fits_key_write_wcsstr (fitsfile ‘*fptr’, char ‘*wcsstr’, int ‘nkeyrec’) Write the WCS header string (produced with WCSLIB’s ‘wcshdo’ function) into the CFITSIO ‘fitsfile’ pointer. ‘nkeyrec’ is the number of FITS header keywords in ‘wcsstr’. This function will put a few blank keyword lines along with a comment ‘WCS information’ before writing each keyword record. -- Function: void gal_fits_key_write (fitsfile ‘*fptr’, gal_fits_list_key_t ‘**keylist’) Write the list of keywords in ‘keylist’ into the CFITSIO ‘fitsfile’. -- Function: void gal_fits_key_write_version (fitsfile ‘*fptr’, gal_fits_list_key_t ‘*headers’, char ‘*program_name’) Write or update (all the) keyword(s) in ‘headers’ into the FITS pointer, but also the date, name of your program (‘program_name’), along with the versions of CFITSIO, WCSLIB (when available), GSL, Gnuastro, and (the possible) commit information into the header as described in *note Output headers::. Since the data processing depends on the versions of the libraries you have used, it is strongly recommended to include this information in every FITS output. ‘gal_fits_img_write’ and ‘gal_fits_tab_write’ will automatically use this function.  File: gnuastro.info, Node: FITS arrays, Next: FITS tables, Prev: FITS header keywords, Up: FITS files 10.3.8.5 FITS arrays (images) ............................. Images (or multi-dimensional arrays in general) are one of the common data formats that is stored in FITS files. Only one image may be stored in each FITS HDU/extension. The functions described here can be used to get the information of, read, or write images in FITS files. -- Function: void gal_fits_img_info (fitsfile ‘*fptr’, int ‘*type’, size_t ‘*ndim’, size_t ‘**dsize’, char ‘**name’, char ‘**unit’) Read the type (see *note Library data types::), number of dimensions, and size along each dimension of the CFITSIO ‘fitsfile’ into the ‘type’, ‘ndim’, and ‘dsize’ pointers respectively. If ‘name’ and ‘unit’ are not ‘NULL’ (point to a ‘char *’), then if the image has a name and units, the respective string will be put in these pointers. -- Function: gal_data_t * gal_fits_img_read (char ‘*filename’, char ‘*hdu’, size_t ‘minmapsize’, size_t ‘hstartwcs’, size_t ‘hendwcs’) Read the contents of the ‘hdu’ extension/HDU of ‘filename’ into a Gnuastro generic data container (see *note Generic data container::) and return it. If the necessary space is larger than ‘minmapsize’, then don’t keep the data in RAM, but in a file on the HDD/SSD. For more on ‘minmapsize’ see the description under the same name in *note Generic data container::. The ‘hstartwcs’ and ‘hendwcs’ arguments are the starting and ending header keywords to search for WCS information, if no limit is needed, set them to zero. For more on these two options, please see the description of ‘gal_wcs_read_fitsptr’ in *note World Coordinate System::. -- Function: gal_data_t * gal_fits_img_read_to_type (char ‘*inputname’, char ‘*inhdu’, uint8_t ‘type’, size_t ‘minmapsize’, ) Read the contents of the ‘hdu’ extension/HDU of ‘filename’ into a Gnuastro generic data container (see *note Generic data container::) of type ‘type’ and return it. This is just a wrapper around ‘gal_fits_img_read’ (to read the image/array of any type) and ‘gal_data_copy_to_new_type_free’ (to convert it to ‘type’ and free the initially read dataset). See the description there for more. -- Function: gal_data_t * gal_fits_img_read_kernel (char ‘*filename’, char ‘*hdu’, size_t ‘minmapsize’) Read the ‘hdu’ of ‘filename’ as a convolution kernel. A convolution kernel must have an odd size along all dimensions, it must not have blank (NaN in floating point types) values and must be flipped around the center to make the proper convolution (see *note Convolution process::). If there are blank values, this function will change the blank values to ‘0.0’. If the input image doesn’t have the other two requirements, this function will abort with an error describing the condition to the user. The finally returned dataset will have a ‘float32’ type. -- Function: fitsfile * gal_fits_img_write_to_ptr (gal_data_t ‘*input’, char ‘*filename’) Write the ‘input’ dataset into a FITS file named ‘filename’ and return the corresponding CFITSIO ‘fitsfile’ pointer. This function won’t close ‘fitsfile’, so you can still add other extensions to it after this function or make other modifications. -- Function: void gal_fits_img_write (gal_data_t ‘*data’, char ‘*filename’, gal_fits_list_key_t ‘*headers’, char ‘*program_string’) Write the ‘input’ dataset into the FITS file named ‘filename’. Also add the ‘headers’ keywords to the newly created HDU/extension it along with your program’s name (‘program_string’). -- Function: void gal_fits_img_write_to_type (gal_data_t ‘*data’, char ‘*filename’, gal_fits_list_key_t ‘*headers’, char ‘*program_string’, int ‘type’) Convert the ‘input’ dataset into ‘type’, then write it into the FITS file named ‘filename’. Also add the ‘headers’ keywords to the newly created HDU/extension along with your program’s name (‘program_string’). After the FITS file is written, this function will free the copied dataset (with type ‘type’) from memory. This is just a wrapper for the ‘gal_data_copy_to_new_type’ and ‘gal_fits_img_write’ functions. -- Function: void gal_fits_img_write_corr_wcs_str (gal_data_t ‘*data’, char ‘*filename’, char ‘*wcsstr’, int ‘nkeyrec’, double ‘*crpix’, gal_fits_list_key_t ‘*headers’, char ‘*program_string’) Write the ‘input’ dataset into ‘filename’ using the ‘wcsstr’ while correcting the ‘CRPIX’ values. This function is mainly useful when you want to make FITS files in parallel (from one main WCS structure, with just differing CRPIX). This can happen in the following cases for example: • When a large number of FITS images (with WCS) need to be created in parallel, it can be much more efficient to write the header’s WCS keywords once at first, write them in the FITS file, then just correct the CRPIX values. • WCSLIB’s header writing function is not thread safe. So when writing FITS images in parallel, we can’t write the header keywords in each thread.  File: gnuastro.info, Node: FITS tables, Prev: FITS arrays, Up: FITS files 10.3.8.6 FITS tables .................... Tables are one of the common formats of data that is stored in FITS files. Only one table may be stored in each FITS HDU/extension, but each table column must be viewed as a different dataset (with its own name, units and numeric data type for example). The only constraint of the column datasets in a table is that they must be one-dimensional and have the same number of elements as the other columns. The functions described here can be used to get the information of, read, or write columns into FITS tables. -- Function: void gal_fits_tab_size (fitsfile ‘*fitsptr’, size_t ‘*nrows’, size_t ‘*ncols’) Read the number of rows and columns in the table within CFITSIO’s ‘fitsptr’. -- Function: int gal_fits_tab_format (fitsfile ‘*fitsptr’) Return the format of the FITS table contained in CFITSIO’s ‘fitsptr’. Recall that FITS tables can be in binary or ASCII formats. This function will return ‘GAL_TABLE_FORMAT_AFITS’ or ‘GAL_TABLE_FORMAT_BFITS’ (defined in *note Table input output::). If the ‘fitsptr’ is not a table, this function will abort the program with an error message informing the user of the problem. -- Function: gal_data_t * gal_fits_tab_info (char ‘*filename’, char ‘*hdu’, size_t ‘*numcols’, size_t ‘*numrows’, int ‘*tableformat’) Store the information of each column in ‘hdu’ of ‘filename’ into an array of data structures with ‘numcols’ elements (one data structure for each column) see *note Arrays of datasets::. The total number of rows in the table is also put into the memory that ‘numrows’ points to. The format of the table (e.g., FITS binary or ASCII table) will be put in ‘tableformat’ (macros defined in *note Table input output::). This function is just for column information. Therefore it only stores meta-data like column name, units and comments. No actual data (contents of the columns for example the ‘array’ or ‘dsize’ elements) will be allocated by this function. This is a low-level function particular to reading tables in FITS format. To be generic, it is recommended to use ‘gal_table_info’ which will allow getting information from a variety of table formats based on the filename (see *note Table input output::). -- Function: gal_data_t * gal_fits_tab_read (char ‘*filename’, char ‘*hdu’, size_t ‘numrows’, gal_data_t ‘*colinfo’, gal_list_sizet_t ‘*indexll’, int ‘minmapsize’) Read the columns given in the list ‘indexll’ from a FITS table into a linked list of data structures, see *note List of size_t:: and *note List of gal_data_t::. If the necessary space for each column is larger than ‘minmapsize’, don’t keep it in the RAM, but in a file in the HDD/SSD, see the description under the same name in *note Generic data container::. Note that this is a low-level function, so the output data linked list is the inverse of the input indexs linked list. It is recommended to use ‘gal_table_read’ for generic reading of tables, see *note Table input output::. -- Function: void gal_fits_tab_write (gal_data_t ‘*cols’, gal_list_str_t ‘*comments’, int ‘tableformat’, char ‘*filename’) Write the list of datasets in ‘cols’ (see *note List of gal_data_t::) as separate columns in a FITS table in ‘filename’. If ‘filename’ already exists then this function will write the table as a new extension after all existing ones. The format of the table (ASCII or binary) may be specified with the ‘tableformat’ (see *note Table input output::). If ‘comments!=NULL’, each node of the list of strings will be written as a ‘COMMENT’ keywords in the output FITS file (see *note List of strings::. This is a low-level function for tables. It is recommended to use ‘gal_table_write’ for generic writing of tables in a variety of formats, see *note Table input output::.  File: gnuastro.info, Node: World Coordinate System, Next: Text files, Prev: FITS files, Up: Gnuastro library 10.3.9 World Coordinate System (‘wcs.h’) ---------------------------------------- The FITS standard defines the world coordinate system (WCS) as a mechanism to associate physical values to positions within a dataset. For example, it can be used to convert pixel coordinates in an image to celestial coordinates like the right ascension and declination. The functions in this section are mainly just wrappers over CFITSIO, WCSLIB and GSL library functions to help in common applications. -- Function: struct wcsprm * gal_wcs_read_fitsptr (fitsfile ‘*fptr’, size_t ‘hstartwcs’, size_t ‘hendwcs’, int ‘*nwcs’) [*Not thread-safe*] Return the WCSLIB ‘wcsprm’ structure that is read from the CFITSIO ‘fptr’ pointer to an opened FITS file. Also put the number of coordinate representations found into the space that ‘nwcs’ points to. To read the WCS structure directly from a filename, see ‘gal_wcs_read’ below. After processing has finished, you can free the returned structure with WCSLIB’s ‘wcsvfree’ keyword: status = wcsvfree(&nwcs,&wcs); If you don’t want to search the full FITS header for WCS-related FITS keywords (for example due to conflicting keywords), but only a specific range of the header keywords you can use the ‘hstartwcs’ and ‘hendwcs’ arguments to specify the keyword number range (counting from zero). If ‘hendwcs’ is larger than ‘hstartwcs’, then only keywords in the given range will be checked. Hence, to ignore this feature (and search the full FITS header), give both these arguments the same value. If the WCS information couldn’t be read from the FITS file, this function will return a ‘NULL’ pointer and put a zero in ‘nwcs’. A WCSLIB error message will also be printed in ‘stderr’ if there was an error. This function is just a wrapper over WCSLIB’s ‘wcspih’ function which is not thread-safe. Therefore, be sure to not call this function simultaneously (over multiple threads). -- Function: struct wcsprm * gal_wcs_read (char ‘*filename’, char ‘*hdu’, size_t ‘hstartwcs’, size_t ‘hendwcs’, int ‘*nwcs’) [*Not thread-safe*] Return the WCSLIB structure that is read from the HDU/extension ‘hdu’ of the file ‘filename’. Also put the number of coordinate representations found into the space that ‘nwcs’ points to. Please see ‘gal_wcs_read_fitsptr’ for more. -- Function: struct wcsprm * gal_wcs_copy (struct wcsprm ‘*wcs’) Return a fully allocated (independent) copy of ‘wcs’. -- Function: void gal_wcs_on_tile (gal_data_t ‘*tile’) Create a WCSLIB ‘wcsprm’ structure for ‘tile’ using WCS parameters of the tile’s allocated block dataset, see *note Tessellation library:: for the definition of tiles. If ‘tile’ already has a WCS structure, this function won’t do anything. In many cases, tiles are created for internal/low-level processing. Hence for performance reasons, when creating the tiles they don’t have any WCS structure. When needed, this function can be used to add a WCS structure to each tile tile by copying the WCS structure of its block and correcting the reference point’s coordinates within the tile. -- Function: double * gal_wcs_warp_matrix (struct wcsprm ‘*wcs’) Return the Warping matrix of the given WCS structure as an array of double precision floating points. This will be the final matrix, irrespective of the type of storage in the WCS structure. Recall that the FITS standard has several methods to store the matrix. The output is an allocated square matrix with each side equal to the number of dimensions. -- Function: void gal_wcs_decompose_pc_cdelt (struct wcsprm ‘*wcs’) Decompose the ‘PCi_j’ and ‘CDELTi’ elements of ‘wcs’. According to the FITS standard, in the ‘PCi_j’ WCS formalism, the rotation matrix elements $m_{ij}$ are encoded in the ‘PCi_j’ keywords and the scale factors are encoded in the ‘CDELTi’ keywords. There is also another formalism (the ‘CDi_j’ formalism) which merges the two into one matrix. However, WCSLIB’s internal operations are apparently done in the ‘PCi_j’ formalism. So its outputs are also all in that format by default. When the input is a ‘CDi_j’, WCSLIB will still read the matrix directly into the ‘PCi_j’ matrix and the ‘CDELTi’ values are set to ‘1’ (one). This function is designed to correct such issues: after it is finished, the ‘CDELTi’ values in ‘wcs’ will correspond to the pixel scale, and the ‘PCi_j’ will correction show the rotation. -- Function: double gal_wcs_angular_distance_deg (double ‘r1’, double ‘d1’, double ‘r2’, double ‘d2’) Return the angular distance (in degrees) between a point located at (‘r1’, ‘d1’) to (‘r2’, ‘d2’). All input coordinates are in degrees. The distance (along a great circle) on a sphere between two points is calculated with the equation below. $$\cos(d)=\sin(d_1)\sin(d_2)+\cos(d_1)\cos(d_2)\cos(r_1-r_2)$$ However, since the the pixel scales are usually very small numbers, this function won’t use that direct formula. It will be use the Haversine formula (https://en.wikipedia.org/wiki/Haversine_formula) which is better considering floating point errors: $${\sin^2(d)\over 2}=\sin^2\left( {d_1-d_2\over 2} \right)+\cos(d_1)\cos(d_2)\sin^2\left( {r_1-r_2\over 2} \right)$$ -- Function: double * gal_wcs_pixel_scale (struct wcsprm ‘*wcs’) Return the pixel scale for each dimension of ‘wcs’ in degrees. The output is an array of double precision floating point type with one element for each dimension. -- Function: double gal_wcs_pixel_area_arcsec2 (struct wcsprm ‘*wcs’) Return the pixel area of ‘wcs’ in arcsecond squared. If the input WCS structure is not two dimensional and the units (‘CUNIT’ keywords) are not ‘deg’ (for degrees), then this function will return a NaN. -- Function: gal_data_t * gal_wcs_world_to_img (gal_data_t ‘*coords’, struct wcsprm ‘*wcs’, int ‘inplace’) Convert the linked list of world coordinates in ‘coords’ to a linked list of image coordinates given the input WCS structure. ‘coords’ must be a linked list of data structures of float64 (‘double’) type, see*note Linked lists:: and *note List of gal_data_t::. The top (first popped/read) node of the linked list must be the first WCS coordinate (RA in an image usually) and etc. Similarly, the top node of the output will be the first image coordinate (in the FITS standard). If ‘inplace’ is zero, then the output will be a newly allocated list and the input list will be untouched. However, if ‘inplace’ is non-zero, the output values will be written into the input’s already allocated array and the returned pointer will be the same pointer to ‘coords’ (in other words, you can ignore the returned value). Note that in the latter case, only the values will be changed, things like units or name (if present) will be untouched. -- Function: gal_data_t * gal_wcs_img_to_world (gal_data_t ‘*coords’, struct wcsprm ‘*wcs’, int ‘inplace’) Convert the linked list of image coordinates in ‘coords’ to a linked list of world coordinates given the input WCS structure. See the description of ‘gal_wcs_world_to_img’ for more details.  File: gnuastro.info, Node: Text files, Next: Table input output, Prev: World Coordinate System, Up: Gnuastro library 10.3.10 Text files (‘txt.h’) ---------------------------- FITS files are the primary data container in astronomy. FITS indeed as many useful features, but the most universal and portable format for data storage are plain text files. They can be viewed and edited on any text editor or even on the command-line. Therefore the functions in this section are defined to simplify reading from and writing to plain text files. Lines are one of the most basic buiding blocks (delimiters) of a text file. Some operating systems like Microsoft Windows, terminate their ASCII text lines with a carriage return character and a new-line character (two characters, also known as CRLF line terminators). While Unix-like operating systems just use a single new-line character. The functions below that read an ASCII text file are able to identify lines with both kinds of line terminators. Gnuastro defines a simple format for metadata of table columns in a plain text file that is discussed in *note Gnuastro text table format::. The functions to get information from, read from and write to plain text files also follow those conventions. -- Macro: GAL_TXT_LINESTAT_INVALID -- Macro: GAL_TXT_LINESTAT_BLANK -- Macro: GAL_TXT_LINESTAT_COMMENT -- Macro: GAL_TXT_LINESTAT_DATAROW Status codes for lines in a plain text file that are returned by ‘gal_txt_line_stat’. Lines which have a <#> character as their first non-white character are considered to be comments. Lines with nothing but white space characters are considered blank. The remaining lines are considered as containing data. -- Function: int gal_txt_line_stat (char ‘*line’) Check the contents of ‘line’ and see if it is a blank, comment, or data line. The returned values are the macros that start with ‘GAL_TXT_LINESTAT’. -- Function: gal_data_t * gal_txt_table_info (char ‘*filename’, size_t ‘*numcols’, size_t ‘*numrows’) Store the information of each column in ‘filename’ into an array of data structures with ‘numcols’ elements (one data structure for each column) see *note Arrays of datasets::. The total number of rows in the table is also put into the memory that ‘numrows’ points to. This function is just for column information. Therefore it only stores meta-data like column name, units and comments. No actual data (contents of the columns for example the ‘array’ or ‘dsize’ elements) will be allocated by this function. This is a low-level function particular to reading tables in plain text format. To be generic, it is recommended to use ‘gal_table_info’ which will allow getting information from a variety of table formats based on the filename (see *note Table input output::). -- Function: gal_data_t * gal_txt_table_read (char ‘*filename’, size_t ‘numrows’, gal_data_t ‘*colinfo’, gal_list_sizet_t ‘*indexll’, size_t ‘minmapsize’) Read the columns given in the list ‘indexll’ from a plain text table into a linked list of data structures, see *note List of size_t:: and *note List of gal_data_t::. If the necessary space for each column is larger than ‘minmapsize’, don’t keep it in the RAM, but in a file on the HDD/SSD, see the description under the same name in *note Generic data container::. Note that this is a low-level function, so the output data list is the inverse of the input indexs linked list. It is recommended to use ‘gal_table_read’ for generic reading of tables in any format, see *note Table input output::. -- Function: gal_data_t * gal_txt_image_read (char ‘*filename’, size_t ‘minmapsize’) Read the 2D plain text dataset in ‘filename’ into a dataset and return the dataset. If the necessary space for the image is larger than ‘minmapsize’, don’t keep it in the RAM, but in a file on the HDD/SSD, see the description under the same name in *note Generic data container::. -- Function: void gal_txt_write (gal_data_t ‘*cols’, gal_list_str_t ‘*comment’, char ‘*filename’) Write ‘cols’ in a plain text file ‘filename’. ‘cols’ may have one or two dimensions which determines the output: 1D ‘cols’ is treated as a column and a list of datasets (see *note List of gal_data_t::): every node in the list is written as one column in a table. 2D ‘cols’ is a two dimensional array, it cannot be treated as a list (only one 2D array can currently be written to a text file). So if ‘cols->next!=NULL’ the next nodes in the list are ignored and will not be written. If ‘filename’ already exists this function will abort with an error and will not write over the existing file. Please make sure if the file exists or not and take the appropriate action before calling this function. If ‘comments!=NULL’, a ‘#’ will be put at the start of each node of the list of strings and will be written in the file before the column meta-data in ‘filename’ (see *note List of strings::). This is a low-level function for tables. It is recommended to use ‘gal_table_write’ for generic writing of tables in a variety of formats, see *note Table input output::.  File: gnuastro.info, Node: Table input output, Next: Arithmetic on datasets, Prev: Text files, Up: Gnuastro library 10.3.11 Table input output (‘table.h’) -------------------------------------- Tables are a collection of one dimensional datasets that are packed together into one file. They are the single most common format to store high-level (processed) information, hence they play a very important role in Gnuastro. For a more thorough introduction, please see *note Table::. Gnuastro’s Table program, and all the other programs that can read from and write into tables, use the functions of this section for reading and writing their input/output tables. For a simple demonstration of using the constructs introduced here, see *note Library demo - reading and writing table columns::. Currently only plain text (see *note Gnuastro text table format::) and FITS (ASCII and binary) tables are supported by Gnuastro. However, the low-level table infra-structure is written such that accommodating other formats is also possible and in future releases more formats will hopefully be supported. Please don’t hesitate to suggest your favorite format so it can be implemented when possible. -- Macro: GAL_TABLE_DEF_WIDTH_STR -- Macro: GAL_TABLE_DEF_WIDTH_INT -- Macro: GAL_TABLE_DEF_WIDTH_LINT -- Macro: GAL_TABLE_DEF_WIDTH_FLT -- Macro: GAL_TABLE_DEF_WIDTH_DBL -- Macro: GAL_TABLE_DEF_PRECISION_INT -- Macro: GAL_TABLE_DEF_PRECISION_FLT -- Macro: GAL_TABLE_DEF_PRECISION_DBL The default width and precision for generic types to use in writing numeric types into a text file (plain text and FITS ASCII tables). When the dataset doesn’t have any pre-set width and precision (see ‘disp_width’ and ‘disp_precision’ in *note Generic data container::) these will be directly used in C’s ‘printf’ command to write the number as a string. -- Macro: GAL_TABLE_DISPLAY_FMT_STRING -- Macro: GAL_TABLE_DISPLAY_FMT_DECIMAL -- Macro: GAL_TABLE_DISPLAY_FMT_UDECIMAL -- Macro: GAL_TABLE_DISPLAY_FMT_OCTAL -- Macro: GAL_TABLE_DISPLAY_FMT_HEX -- Macro: GAL_TABLE_DISPLAY_FMT_FLOAT -- Macro: GAL_TABLE_DISPLAY_FMT_EXP -- Macro: GAL_TABLE_DISPLAY_FMT_GENERAL The display format used in C’s ‘printf’ to display data of different types. The ‘_STRING’ and ‘_DECIMAL’ are unique for printing strings and signed integers, they are mainly here for completeness. However, unsigned integers and floating points can be displayed in multiple formats: Unsigned integer For unsigned integers, it is possible to choose from ‘_UDECIMAL’ (unsigned decimal), ‘_OCTAL’ (octal notation, for example ‘125’ in decimal will be displayed as ‘175’), and ‘_HEX’ (hexadecimal notation, for example ‘125’ in decimal will be displayed as ‘7D’). Floating point For floating point, it is possible to display the number in ‘_FLOAT’ (floating point, for example ‘1500.345’), ‘_EXP’ (exponential, for example ‘1.500345e+03’), or ‘_GENERAL’ which is the best of the two for the given number. -- Macro: GAL_TABLE_FORMAT_INVALID -- Macro: GAL_TABLE_FORMAT_TXT -- Macro: GAL_TABLE_FORMAT_AFITS -- Macro: GAL_TABLE_FORMAT_BFITS All the current acceptable table formats to Gnuastro. The ‘AFITS’ and ‘BFITS’ represent FITS ASCII tables and FITS Binary tables. You can use these anywhere you see the ‘tableformat’ variable. -- Macro: GAL_TABLE_SEARCH_INVALID -- Macro: GAL_TABLE_SEARCH_NAME -- Macro: GAL_TABLE_SEARCH_UNIT -- Macro: GAL_TABLE_SEARCH_COMMENT When the desired column is not a number, these values determine if the string to match, or regular expression to search, be in the _name_, _units_ or _comments_ of the column meta data. These values should be used for the ‘searchin’ variables of the functions. -- Function: gal_data_t * gal_table_info (char ‘*filename’, char ‘*hdu’, size_t ‘*numcols’, size_t ‘*numrows’, int ‘*tableformat’) Store the information of each column in a table (either as a text file or as a FITS table) into an array of data structures with ‘numcols’ structures (one data structure for each column). The number of rows is stored in the space that ‘numrows’ points to. The format of the table (e.g., ascii text file, or FITS binary or ASCII table) will be put in ‘tableformat’ (macros defined above). If the filename is not a FITS file, then ‘hdu’ will not be used (can be ‘NULL’). Note that other than the character strings (column name, units and comments), nothing in the data structure(s) will be allocated by this function for the actual data (e.g., the ‘array’ or ‘dsize’ elements). This function is just for column information (meta-data), not column contents. -- Function: void gal_table_print_info (gal_data_t ‘*allcols’, size_t ‘numcols’, size_t ‘numrows’) This program will print the column information for all the columns (output of ‘gal_table_info’). The output is in the same format as this command with Gnuastro Table program (see *note Table::): $ asttable --info table.fits -- Function: gal_data_t * gal_table_read (char ‘*filename’, char ‘*hdu’, gal_list_str_t ‘*cols’, int ‘searchin’, int ‘ignorecase’, int ‘minmapsize’, size_t ‘colmatch’) Read the specified columns in a text file (named ‘filename’) into a linked list of data structures. If the file is FITS, then ‘hdu’ will also be used, otherwise, ‘hdu’ is ignored. The information to search for columns should be specified by the ‘cols’ list of strings (see *note List of strings::). The string in each node of the list may be a number, an exact match to a column name, or a regular expression (in GNU AWK format) enclosed in ‘/ /’. The ‘searchin’ value must be one of the macros defined above. If ‘cols’ is NULL, then this function will read the full table. The output is an individually allocated list of datasets (see *note List of gal_data_t::) with the same order of the ‘cols’ list. Note that one column node in the ‘cols’ list might give multiple columns (for example from regular expressions), in this case, the order of output columns that correspond to that one input, are in order of the table (which column was read first). So the first requested column is the first popped data structure and so on. if ‘colmatch!=NULL’, it is assumed to be an array that has at least the same number of elements as nodes in the ‘cols’ list. The number of columns that matched each input column will be stored in each element. -- Function: void gal_table_comments_add_intro (gal_list_str_t ‘**comments’, char ‘*program_string’, time_t ‘*rawtime’) Add some basic information to the list of ‘comments’. This basic information includes the following information • If the program is run in a Git version controlled directory, Git’s description is printed (see description under ‘COMMIT’ in *note Output headers::). • The calendar time that is stored in ‘rawtime’ (‘time_t’ is C’s calendar time format defined in ‘time.h’). You can calculate the time in this format with the following expressions: time_t rawtime; time(&rawtime); • The name of your program in ‘program_string’. If it is ‘NULL’, this line is ignored. -- Function: void gal_table_write (gal_data_t ‘*cols’, gal_list_str_t ‘*comments’, int ‘tableformat’, char ‘*filename’, char ‘*extname’) Write the ‘cols’ list of datasets into a table in ‘filename’ (see *note List of gal_data_t::). The format of the table can be determined with ‘tableformat’ that accepts the macros defined above. If ‘comments’ is not ‘NULL’, then the list of comments will also be printed into the output table. When the output table is a plain text file, each node’s string will be printed after a ‘#’ (so it can be considered as a comment) and in FITS table they will follow a ‘COMMENT’ keyword. If ‘filename’ is a FITS file, the table extension that will be written will have the name ‘extname’. If a file named ‘filename’ already exists, the operation depends on the type of output. When ‘filename’ is a FITS file, the table will be added as a new extension after all existing ones. If ‘filename’ is a plain text file, this function will abort with an error. -- Function: void gal_table_write_log (gal_data_t ‘*logll’, char ‘*program_string’, time_t ‘*rawtime’, gal_list_str_t ‘*comments’, char ‘*filename’, int ‘quiet’) Write the ‘logll’ list of datasets into a table in ‘filename’ (see *note List of gal_data_t::). This function is just a wrapper around ‘gal_table_comments_add_intro’ and ‘gal_table_write’ (see above). If ‘quiet’ is non-zero, this function will print a message saying that the ‘filename’ has been created.  File: gnuastro.info, Node: Arithmetic on datasets, Next: Tessellation library, Prev: Table input output, Up: Gnuastro library 10.3.12 Arithmetic on datasets (‘arithmetic.h’) ----------------------------------------------- When the dataset’s type and other information are already known, any programming language (including C) provides some very good tools for various operations (including arithmetic operations like addition) on the dataset with a simple loop. However, as an author of a program, making assumptions about the type of data, its dimensions and other basic characteristics will come with a large processing burden. For example if you always read your data as double precision floating points for a simple operation like addition with an integer constant, you will be wasting a lot of CPU and memory when the input dataset is ‘int32’ type for example (see *note Numeric data types::). This overhead may be small for small images, but as you scale your process up and work with hundred/thousands of files that can be very large, this overhead will take a significant portion of the processing power. The functions and macros in this section are designed precisely for this purpose: to allow you to do any of the defined operations on any dataset with no overhead (in the native type of the dataset). Gnuastro’s Arithmetic program uses the functions and macros of this section, so please also have a look at the *note Arithmetic:: program and in particular *note Arithmetic operators:: for a better description of the operators discussed here. The main function of this library is ‘gal_arithmetic’ that is described below. It can take an arbitrary number of arguments as operands (depending on the operator, similar to ‘printf’). Its first two arguments are integers specifying the flags and operator. So first we will review the constants for the recognized flags and operators and discuss them, then introduce the actual function. -- Macro: GAL_ARITHMETIC_INPLACE -- Macro: GAL_ARITHMETIC_FREE -- Macro: GAL_ARITHMETIC_NUMOK -- Macro: GAL_ARITHMETIC_FLAGS_ALL Bit-wise flags to pass onto ‘gal_arithmetic’ (see below). To pass multiple flags, use the bitwise-or operator, for example ‘GAL_ARITHMETIC_INPLACE | GAL_ARITHMETIC_FREE’. ‘GAL_ARITHMETIC_FLAGS_ALL’ is a combination of all flags to shorten your code if you want all flags activated. Each flag is described below: ‘GAL_ARITHMETIC_INPLACE’ Do the operation in-place (in the input dataset, thus modifying it) to improve CPU and memory usage. If this flag is used, after ‘gal_arithmetic’ finishes, the input dataset will be modified. It is thus useful if you have no more need for the input after the operation. ‘GAL_ARITHMETIC_FREE’ Free (all the) input dataset(s) after the operation is done. Hence the inputs are no longer usable after ‘gal_arithmetic’. ‘GAL_ARITHMETIC_NUMOK’ It is acceptable to use a number and an array together. For example if you want to add all the pixels in an image with a single number you can pass this flag to avoid having to allocate a constant array the size of the image (with all the pixels having the same number). -- Macro: GAL_ARITHMETIC_OP_PLUS -- Macro: GAL_ARITHMETIC_OP_MINUS -- Macro: GAL_ARITHMETIC_OP_MULTIPLY -- Macro: GAL_ARITHMETIC_OP_DIVIDE -- Macro: GAL_ARITHMETIC_OP_LT -- Macro: GAL_ARITHMETIC_OP_LE -- Macro: GAL_ARITHMETIC_OP_GT -- Macro: GAL_ARITHMETIC_OP_GE -- Macro: GAL_ARITHMETIC_OP_EQ -- Macro: GAL_ARITHMETIC_OP_NE -- Macro: GAL_ARITHMETIC_OP_AND -- Macro: GAL_ARITHMETIC_OP_OR Binary operators (requiring two operands) that accept datasets of any recognized type (see *note Numeric data types::). When ‘gal_arithmetic’ is called with any of these operators, it expects two datasets as arguments. For a full description of these operators with the same name, see *note Arithmetic operators::. The first dataset/operand will be put on the left of the operator and the second will be put on the right. The output type of the first four is determined from the input types (largest type of the inputs). The rest (which are all conditional operators) will output a binary ‘uint8_t’ (or ‘unsigned char’) dataset with values of either ‘0’ (zero) or ‘1’ (one). -- Macro: GAL_ARITHMETIC_OP_NOT The logical NOT operator. When ‘gal_arithmetic’ is called with this operator, it only expects one operand (dataset), since this is a unary operator. The output is ‘uint8_t’ (or ‘unsigned char’) dataset of the same size as the input. Any non-zero element in the input will be ‘0’ (zero) in the output and any ‘0’ (zero) will have a value of ‘1’ (one). -- Macro: GAL_ARITHMETIC_OP_ISBLANK A unary operator with output that is ‘1’ for any element in the input that is blank, and ‘0’ for any non-blank element. When ‘gal_arithmetic’ is called with this operator, it will only expect one input dataset. The output dataset will have ‘uint8_t’ (or ‘unsigned char’) type. ‘gal_arithmetic’ with this operator is just a wrapper for the ‘gal_blank_flag’ function of *note Library blank values:: and this operator is just included for completeness in arithmetic operations. So in your program, it might be easier to just call ‘gal_blank_flag’. -- Macro: GAL_ARITHMETIC_OP_WHERE The three-operand _where_ operator thoroughly discussed in *note Arithmetic operators::. When ‘gal_arithmetic’ is called with this operator, it will only expect three input datasets: the first (which is the same as the returned dataset) is the array that will be modified. The second is the condition dataset (that must have a ‘uint8_t’ or ‘unsigned char’ type), and the third is the value to be used if condition is non-zero. As a result, note that the order of operands when calling ‘gal_arithmetic’ with ‘GAL_ARITHMETIC_OP_WHERE’ is the opposite of running Gnuastro’s Arithmetic program with the ‘where’ operator (see *note Arithmetic::). This is because the latter uses the reverse-Polish notation which isn’t necessary when calling a function (see *note Reverse polish notation::). -- Macro: GAL_ARITHMETIC_OP_SQRT -- Macro: GAL_ARITHMETIC_OP_LOG -- Macro: GAL_ARITHMETIC_OP_LOG10 Unary operator functions for calculating the square root ($\sqrt{i}$), $ln(i)$ and $log(i)$ mathematic operators on each element of the input dataset. The output will have the same type as the input, so if your inputs are integer types be careful. If you want your output to be floating point but your input is an integer type, you can convert the input to a floating point type with ‘gal_data_copy_to_new_type’ or ‘gal_data_copy_to_new_type_free’(see *note Copying datasets::). -- Macro: GAL_ARITHMETIC_OP_MINVAL -- Macro: GAL_ARITHMETIC_OP_MAXVAL -- Macro: GAL_ARITHMETIC_OP_NUMVAL -- Macro: GAL_ARITHMETIC_OP_SUMVAL -- Macro: GAL_ARITHMETIC_OP_MEANVAL -- Macro: GAL_ARITHMETIC_OP_STDVAL -- Macro: GAL_ARITHMETIC_OP_MEDIANVAL Unary operand statistical operators that will return a single value for datasets of any size. These are just wrappers around similar functions in *note Statistical operations:: and are included in ‘gal_arithmetic’ only for completeness (to use easily in *note Arithmetic::). In your programs, it will probably be easier if you use those ‘gal_statistics_’ functions directly. -- Macro: GAL_ARITHMETIC_OP_ABS Unary operand absolute-value operator. -- Macro: GAL_ARITHMETIC_OP_MIN -- Macro: GAL_ARITHMETIC_OP_MAX -- Macro: GAL_ARITHMETIC_OP_NUM -- Macro: GAL_ARITHMETIC_OP_SUM -- Macro: GAL_ARITHMETIC_OP_MEAN -- Macro: GAL_ARITHMETIC_OP_STD -- Macro: GAL_ARITHMETIC_OP_MEDIAN Multi-operand statistical operations. When ‘gal_arithmetic’ is called with any of these operators, it will expect only a single operand that will be interpretted as a list of datasets (see *note List of gal_data_t::. The output will be a single dataset with each of its elements replaced by the respective statistical operation on the whole list. See the discussion under the ‘min’ operator in *note Arithmetic operators::. -- Macro: GAL_ARITHMETIC_OP_POW Binary operator to-power operator. When ‘gal_arithmetic’ is called with any of these operators, it will expect two operands: raising the first by the second. This operator only accepts floating point inputs and the output is also floating point. -- Macro: GAL_ARITHMETIC_OP_BITAND -- Macro: GAL_ARITHMETIC_OP_BITOR -- Macro: GAL_ARITHMETIC_OP_BITXOR -- Macro: GAL_ARITHMETIC_OP_BITLSH -- Macro: GAL_ARITHMETIC_OP_BITRSH -- Macro: GAL_ARITHMETIC_OP_MODULO Binary integer-only operand operators. These operators are only defined on integer data types. When ‘gal_arithmetic’ is called with any of these operators, it will expect two operands: the first is put on the left of the operator and the second on the right. The ones starting with ‘BIT’ are the respective bit-wise operators in C and ‘MODULO’ is the modulo/remainder operator. For a discussion on these operators, please see *note Arithmetic operators::. The output type is determined from the input types and C’s internal conversions: it is strongly recommended that both inputs have the same type (any integer type), otherwise the bit-wise behavior will be determined by your compiler. -- Macro: GAL_ARITHMETIC_OP_BITNOT The unary bit-wise NOT operator. When ‘gal_arithmetic’ is called with any of these operators, it will expect one operand of an integer type and preform the bitwise-NOT operation on it. The output will have the same type as the input. -- Macro: GAL_ARITHMETIC_OP_TO_UINT8 -- Macro: GAL_ARITHMETIC_OP_TO_INT8 -- Macro: GAL_ARITHMETIC_OP_TO_UINT16 -- Macro: GAL_ARITHMETIC_OP_TO_INT16 -- Macro: GAL_ARITHMETIC_OP_TO_UINT32 -- Macro: GAL_ARITHMETIC_OP_TO_INT32 -- Macro: GAL_ARITHMETIC_OP_TO_UINT64 -- Macro: GAL_ARITHMETIC_OP_TO_INT64 -- Macro: GAL_ARITHMETIC_OP_TO_FLOAT32 -- Macro: GAL_ARITHMETIC_OP_TO_FLOAT64 Unary type-conversion operators. When ‘gal_arithmetic’ is called with any of these operators, it will expect one operand and convert it to the requested type. Note that with these operators, ‘gal_arithmetic’ is just a wrapper over the ‘gal_data_copy_to_new_type’ or ‘gal_data_copy_to_new_type_free’ that are discussed in ‘Copying datasets’. It accepts these operators only for completeness and easy usage in *note Arithmetic::. So in your programs, it might be preferable to directly use those functions. -- Function: gal_data_t * gal_arithmetic (int operator, int flags, ...) Do the arithmetic operation of ‘operator’ on the given operands (the third argument and any further argument). Certain special conditions can also be specified with the ‘flag’ operator. The acceptable values for ‘operator’ are defined in the macros above. ‘gal_arithmetic’ is a multi-argument function (like C’s ‘printf’). In other words, the number of necessary arguments is not fixed and depends on the value to ‘operator’. Here are a few examples showing this variability: out_1=gal_arithmetic(GAL_ARITHMETIC_OP_LOG, 0, in_1); out_2=gal_arithmetic(GAL_ARITHMETIC_OP_PLUS, 0, in_1, in_2); out_3=gal_arithmetic(GAL_ARITHMETIC_OP_WHERE, 0, in_1, in_2, in_3); The number of necessary operands for each operator (and thus the number of necessary arguments to ‘gal_arithmetic’) are described above under each operator.  File: gnuastro.info, Node: Tessellation library, Next: Bounding box, Prev: Arithmetic on datasets, Up: Gnuastro library 10.3.13 Tessellation library (‘tile.h’) --------------------------------------- In many contexts, it is desirable to slice the dataset into subsets or tiles (overlapping or not). In such a way that you can work on each tile independently. One method would be to copy that region to a separate allocated space, but in many contexts this isn’t necessary and in fact can be a big burden on CPU/Memory usage. The ‘block’ pointer in Gnuastro’s *note Generic data container:: is defined for such situations: where allocation is not necessary. You just want to read the data or write to it independently (or in coordination with) other regions of the dataset. Added with parallel processing, this can greatly improve the time/memory consumption. See the figure below for example: assume the ‘larger’ dataset is a contiguous block of memory that you are interpreting as a 2D array. But you only want to work on the smaller ‘tile’ region. larger --------------------------------- | | | tile | | ---------- | | | | | | |_ | | | |*| | | | ---------- | | tile->block = larger | |_ | |*| | --------------------------------- To use ‘gal_data_t’’s ‘block’ concept, you allocate a ‘gal_data_t *tile’ which is initialized with the pointer to the first element in the sub-array (as its ‘array’ argument). Note that this is not necessarily the first element in the larger array. You can set the size of the tile along with the initialization as you please. Recall that, when given a non-‘NULL’ pointer as ‘array’, ‘gal_data_initialize’ (and thus ‘gal_data_alloc’) do not allocate any space and just uses the given pointer for the new ‘array’ element of the ‘gal_data_t’. So your ‘tile’ data structure will not be pointing to a separately allocated space. After the allocation is done, you just point ‘tile->block’ to the ‘larger’ dataset which hosts the full block of memory. Where relevant, Gnuastro’s library functions will check the ‘block’ pointer of their input dataset to see how to deal with dimensions and increments so they can always remain within the tile. The tools introduced in this section are designed to help in defining and working with tiles that are created in this manner. Since the block structure is defined as a pointer, arbitrary levels of tessellation/grid-ing are possible (‘tile->block’ may itself be a tile in an even larger allocated space). Therefore, just like a linked-list (see *note Linked lists::), it is important to have the ‘block’ pointer of the largest (allocated) dataset set to ‘NULL’. Normally, you won’t have to worry about this, because ‘gal_data_initialize’ (and thus ‘gal_data_alloc’) will set the ‘block’ element to ‘NULL’ by default, just remember not to change it. You can then only change the ‘block’ element for the tiles you define over the allocated space. Below, we will first review constructs for *note Independent tiles:: and then define the current approach to fully tessellating a dataset (or covering every pixel/data-element with a non-overlapping tile grid in *note Tile grid::. This approach to dealing with parts of a larger block was inspired from a similarly named concept in the GNU Scientific Library (GSL), see its “Vectors and Matrices†chapter for their implementation. * Menu: * Independent tiles:: Work on or check independent tiles. * Tile grid:: Cover a full dataset with non-overlapping tiles.  File: gnuastro.info, Node: Independent tiles, Next: Tile grid, Prev: Tessellation library, Up: Tessellation library 10.3.13.1 Independent tiles ........................... The most general application of tiles is to treat each independently, for example they may overlap, or they may not cover the full image. This section provides functions to help in checking/inspecting such tiles. In *note Tile grid:: we will discuss functions that define/work-with a tile grid (where the tiles don’t overlap and fully cover the input dataset). Therefore, the functions in this section are general and can be used for the tiles produced by that section also. -- Function: void gal_tile_start_coord (gal_data_t ‘*tile’, size_t ‘*start_coord’) Calculate the starting coordinates of a tile in its allocated block of memory and write them in the memory that ‘start_coord’ points to (which must have ‘tile->ndim’ elements). -- Function: void gal_tile_start_end_coord (gal_data_t ‘*tile’, size_t ‘*start_end’, int ‘rel_block’) Put the starting and ending (end point is not inclusive) coordinates of ‘tile’ into the ‘start_end’ array. It is assumed that a space of ‘2*tile->ndim’ has been already allocated (static or dynamic) for ‘start_end’ before this function is called. ‘rel_block’ (or relative-to-block) is only relevant when ‘tile’ has an intermediate tile between it and the allocated space (like a channel, see ‘gal_tile_full_two_layers’). If it doesn’t (‘tile->block’ points the allocated dataset), then the value to ‘rel_block’ is irrelevant. When ‘tile->block’ is its self a larger block and ‘rel_block’ is set to 0, then the starting and ending positions will be based on the position within ‘tile->block’, not the allocated space. -- Function: void * gal_tile_start_end_ind_inclusive (gal_data_t ‘*tile’, gal_data_t ‘*work’, size_t ‘*start_end_inc’) Put the indexs of the first/start and last/end pixels (inclusive) in a tile into the ‘start_end’ array (that must have two elements). NOTE: this function stores the index of each point, not its coordinates. It will then return the pointer to the start of the tile in the ‘work’ data structure (which doesn’t have to be equal to ‘tile->block’. The outputs of this function are defined to make it easy to parse over an n-dimensional tile. For example, this function is one of the most important parts of the internal processing of in ‘GAL_TILE_PARSE_OPERATE’ function-like macro that is described below. -- Function: gal_data_t * gal_tile_series_from_minmax (gal_data_t ‘*block’, size_t ‘*minmax’, size_t ‘number’) Construct a list of tile(s) given coordinates of the minimum and maximum of each tile. The minimum and maximums are assumed to be inclusive. The returned pointer is an allocated ‘gal_data_t’ array that can later be freed with ‘gal_data_array_free’ (see *note Arrays of datasets::). Internally, each element of the output array points to the next element, so the output may also be treated as a list of datasets (see *note List of gal_data_t::) and passed onto the other functions described in this section. The array keeping the minimum and maximum coordinates for each tile must have the following format. So in total ‘minmax’ must have ‘2*ndim*number’ elements. | min0_d0 | min0_d1 | max0_d0 | max0_d1 | ... ... | minN_d0 | minN_d1 | maxN_d0 | maxN_d1 | -- Function: gal_data_t * gal_tile_block (gal_data_t ‘*tile’) Return the dataset that contains ‘tile’’s allocated block of memory. If tile is immediately defined as part of the allocated block, then this is equivalent to ‘tile->block’. However, it is possible to have multiple layers of tiles (where ‘tile->block’ is itself a tile). So this function is the most generic way to get to the actual allocated dataset. -- Function: size_t gal_tile_block_increment (gal_data_t ‘*block’, size_t ‘*tsize’, size_t ‘num_increment’, size_t ‘*coord’) Return the increment necessary to start at the next contiguous patch memory associated with a tile. ‘block’ is the allocated block of memory and ‘tsize’ is the size of the tile along every dimension. If ‘coord’ is ‘NULL’, it is ignored. Otherwise, it will contain the coordinate of the start of the next contiguous patch of memory. This function is intended to be used in a loop and ‘num_increment’ is the main variable to this function. For the first time you call this function, it should be ‘1’. In subsequent calls (while you are parsing a tile), it should be increased by one. -- Function: gal_data_t * gal_tile_block_write_const_value (gal_data_t ‘*tilevalues’, gal_data_t ‘*tilesll’, int ‘withblank’, int ‘initialize’) Write a constant value for each tile over the area it covers in an allocated dataset that is the size of ‘tile’’s allocated block of memory (found through ‘gal_tile_block’ described above). The arguments to this function are: ‘tilevalues’ This must be an array that has the same number of elements as the nodes in in ‘tilesll’ and in the same order that ‘tilesll’ elements are parsed (from top to bottom, see *note Linked lists::). As a result the array’s number of dimensions is irrelevant, it will be parsed contiguously. ‘tilesll’ The list of input tiles (see *note List of gal_data_t::). Internally, it might be stored as an array (for example the output of ‘gal_tile_series_from_minmax’ described above), but this function doesn’t care, it will parse the ‘next’ elements to go to the next tile. This function will not pop-from or free the ‘tilesll’, it will only parse it from start to end. ‘withblank’ If the block containing the tiles has blank elements, those blank elements will be blank in the output of this function also, hence the array will be initialized with blank values when this option is called (see below). ‘initialize’ Initialize the allocated space with blank values before writing in the constant values. This can be useful when the tiles don’t cover the full allocated block. -- Function: gal_data_t * gal_tile_block_check_tiles (gal_data_t ‘*tilesll’) Make a copy of the memory block and fill it with the index of each tile in ‘tilesll’ (counting from 0). The non-filled areas will have blank values. The output dataset will have a type of ‘GAL_TYPE_INT32’ (see *note Library data types::). This function can be used when you want to check the coverage of each tile over the allocated block of memory. It is just a wrapper over the ‘gal_tile_block_write_const_value’ (with ‘withblank’ set to zero). -- Function: void * gal_tile_block_relative_to_other (gal_data_t ‘*tile’, gal_data_t ‘*other’) Return the pointer corresponding to the start of the region covered by ‘tile’ over the ‘other’ dataset. See the examples in ‘GAL_TILE_PARSE_OPERATE’ for some example applications of this function. -- Function: void gal_tile_block_blank_flag (gal_data_t ‘*tilell’, size_t ‘numthreads’) Check if each tile in the list has blank values and update its ‘flag’ to mark this check and its result (see *note Generic data container::). The operation will be done on ‘numthreads’ threads. -- Function-like macro: GAL_TILE_PARSE_OPERATE (‘IN’, ‘OTHER’, ‘PARSE_OTHER’, ‘CHECK_BLANK’, ‘OP’) Parse ‘IN’ (which can be a tile or a fully allocated block of memory) and do the ‘OP’ operation on it. ‘OP’ can be any combination of C expressions. If ‘OTHER!=NULL’, ‘OTHER’ will be interpretted as a dataset and this macro will allow access to its element(s) and it can optionally be parsed while parsing over ‘IN’. If ‘OTHER’ is a fully allocated block of memory (not a tile), then the same region that is covered by ‘IN’ within its own block will be parsed (the same starting pixel with the same number of pixels in each dimension). Hence, in this case, the blocks of ‘OTHER’ and ‘IN’ must have the same size. When ‘OTHER’ is a tile it must have the same size as ‘IN’ and parsing will start from its starting element/pixel. Also, the respective allocated blocks of ‘OTHER’ and ‘IN’ (if different) may have different sizes. Using ‘OTHER’ (along with ‘PARSE_OTHER’), this funciton-like macro will thus enable you to parse and define your own operation on two fixed size regions in one or two blocks of memory. In the latter case, they may have different numeric datatypes, see *note Numeric data types::). The input arguments to this macro are explained below, the expected type of each argument are also written following the argument name: ‘IN (gal_data_t)’ Input dataset, this can be a tile or an allocated block of memory. ‘OTHER (gal_data_t)’ Dataset (‘gal_data_t’) to parse along with ‘IN’. It can be ‘NULL’. In that case, ‘o’ (see description of ‘OP’ below) will be ‘NULL’ and should not be used. If ‘PARSE_OTHER’ is zero, only its first element will be used and the size of this dataset is irrelevant. When ‘OTHER’ is a block of memory, it has to have the same size as the allocated block of ‘IN’. When its a tile, it has to have the same size as ‘IN’. ‘PARSE_OTHER (int)’ Parse the other dataset along with the input. When this is non-zero and ‘OTHER!=NULL’, then the ‘o’ pointer will be incremented to cover the ‘OTHER’ tile at the same rate as ‘i’, see description of ‘OP’ for ‘i’ and ‘o’. ‘CHECK_BLANK (int)’ If it is non-zero, then the input will be checked for blank values and ‘OP’ will only be called when we are not on a blank element. ‘OP’ Operator: this can be any number of C expressions. This macro is going to define a ‘itype *i’ variable which will increment over each element of the input array/tile. ‘itype’ will be replaced with the C type that corresponds to the type of ‘INPUT’. As an example, if ‘INPUT’’s type is ‘GAL_DATA_UINT16’ or ‘GAL_DATA_FLOAT32’, ‘i’ will be defined as ‘uint16’ or ‘float’ respectively. This function-like macro will also define an ‘otype *o’ which you can use to access an element of the ‘OTHER’ dataset (if ‘OTHER!=NULL’). ‘o’ will correspond to the type of ‘OTHER’ (similar to ‘itype’ and ‘INPUT’ discussed above). If ‘PARSE_OTHER’ is non-zero, then ‘o’ will also be incremented to the same index element but in the other array. You can use these along with any other variable you define before this macro to process the input and store it in the other. All variables within this function-like macro begin with ‘tpo_’ except for the three variables listed above. So as long as you don’t start the names of your variables with this prefix everything will be fine. Note that ‘i’ (and possibly ‘o’) will be incremented once by this function-like macro, so don’t increment them within ‘OP’. As a summary, the three variables you have access to within ‘OP’ are: ‘i’ Pointer to the element of ‘INPUT’ that is being parsed with the proper type. ‘o’ Pointer to the element of ‘OTHER’ that is being parsed with the proper type. ‘o’ can only be used if ‘OTHER!=NULL’ and it will be parsed/incremented if ‘PARSE_OTHER’ is non-zero. ‘b’ Blank value in the type of ‘INPUT’. You can use a given tile (‘tile’ on a dataset that it was not initialized with but has the same size, let’s call it ‘new’) with the following steps: void *tarray; gal_data_t *tblock; /* `tile->block' must be corrected AFTER `tile->array'. */ tarray = tile->array; tblock = tile->block; tile->array = gal_tile_block_relative_to_other(tile, new); tile->block = new; /* Parse and operate over this region of the `new' dataset. */ GAL_TILE_PARSE_OPERATE(tile, NULL, 0, 0, { YOUR_PROCESSING; }); /* Reset `tile->block' and `tile->array'. */ tile->array=tarray; tile->block=tblock; You can work on the same region of another block in one run of this function-like macro. To do that, you can make a fake tile and pass that as the ‘OTHER’ argument. Below is a demonstration, ‘tile’ is the actual tile that you start with and ‘new’ is the other block of allocated memory. size_t zero=0; gal_data_t *faketile; /* Allocate the fake tile, these can be done outside a loop * (over many tiles). */ faketile=gal_data_alloc(NULL, new->type, 1, &zero, NULL, 0, -1, NULL, NULL, NULL); free(faketile->array); /* To keep things clean. */ free(faketile->dsize); /* To keep things clean. */ faketile->block = new; faketile->ndim = new->ndim; /* These can be done in a loop (over many tiles). */ faketile->size = tile->size; faketile->dsize = tile->dsize; faketile->array = gal_tile_block_relative_to_other(tile, new); /* Do your processing.... in a loop (over many tiles). */ GAL_TILE_PARSE_OPERATE(tile, faketile, 1, 1, { YOUR_PROCESSING_EXPRESSIONS; }); /* Clean up (outside the loop). */ faketile->array=NULL; faketile->dsize=NULL; gal_data_free(faketile);  File: gnuastro.info, Node: Tile grid, Prev: Independent tiles, Up: Tessellation library 10.3.13.2 Tile grid ................... One very useful application of tiles is to completely cover an input dataset with tiles. Such that you know every pixel/data-element of the input image is covered by only one tile. The constructs in this section allow easy definition of such a tile structure. They will create lists of tiles that are also usable by the general tools discussed in *note Independent tiles::. As discussed in *note Tessellation::, (mainly raw) astronomical images will mostly require two layers of tessellation, one for amplifier channels which all have the same size and another (smaller tile-size) tessellation over each channel. Hence, in this section we define a general structure to keep the main parameters of this two-layer tessellation and help in benefiting from it. -- Type (C ‘struct’): gal_tile_two_layer_params This is the general structure to keep all the necessary parameters for a two-layer tessellation. struct gal_tile_two_layer_params { /* Inputs */ size_t *tilesize; /*******************************/ size_t *numchannels; /* These parameters have to be */ float remainderfrac; /* filled manually before */ uint8_t workoverch; /* calling the functions in */ uint8_t checktiles; /* this section. */ uint8_t oneelempertile; /*******************************/ /* Internal parameters. */ size_t ndim; size_t tottiles; size_t tottilesinch; size_t totchannels; size_t *channelsize; size_t *numtiles; size_t *numtilesinch; char *tilecheckname; size_t *permutation; size_t *firsttsize; /* Tile and channel arrays (which are also lists). */ gal_data_t *tiles; gal_data_t *channels; }; -- Function: size_t * gal_tile_full (gal_data_t ‘*input’, size_t ‘*regular’, float ‘remainderfrac’, gal_data_t ‘**out’, size_t ‘multiple’, size_t ‘**firsttsize’) Cover the full dataset with (mostly) identical tiles and return the number of tiles created along each dimension. The regular tile size (along each dimension) is determined from the ‘regular’ array. If ‘input’’s size is not an exact multiple of ‘regular’ for each dimension, then the tiles touching the edges in that dimension will have a different size to fully cover every element of the input (depending on ‘remainderfrac’). The output is an array with the same dimensions as ‘input’ which contains the number of tiles along each dimension. See *note Tessellation:: for a description of its application in Gnuastro’s programs and ‘remainderfrac’, just note that this function defines only one layer of tiles. This is a low-level function (independent of the ‘gal_tile_two_layer_params’ structure defined above). If you want a two-layer tessellation, directly call ‘gal_tile_full_two_layers’ that is described below. The input arguments to this function are: ‘input’ The main dataset (allocated block) which you want to create a tessellation over (only used for its sizes). So ‘input’ may be a tile also. ‘regular’ The the size of the regular tiles along each of the input’s dimensions. So it must have the same number of elements as the dimensions of ‘input’ (or ‘input->ndim’). ‘remainderfrac’ The significant fraction of the remainder space to see if it should be split into two and put on both sides of a dimension or not. This is thus only relevant ‘input’ length along a dimension isn’t an exact multiple of the regular tile size along that dimension. See *note Tessellation:: for a more thorough discussion. ‘out’ Pointer to the array of data structures that will keep all the tiles (see *note Arrays of datasets::). If ‘*out==NULL’, then the necessary space to keep all the tiles will be allocated. If not, then all the tile information will be filled from the dataset that ‘*out’ points to, see ‘multiple’ for more. ‘multiple’ When ‘*out==NULL’ (and thus will be allocated by this function), allocate space for ‘multiple’ times the number of tiles needed. This can be very useful when you have several more identically sized ‘inputs’, and you want all their tiles to be allocated (and thus indexed) together, even though they have different ‘block’ datasets (that then link to one allocated space). See the definition of channels in *note Tessellation:: and ‘gal_tile_full_two_layers’ below. ‘firsttsize’ The size of the first tile along every dimension. This is only different from the regular tile size when ‘regular’ is not an exact multiple of ‘input’’s length along every dimension. This array is allocated internally by this function. -- Function: void gal_tile_full_sanity_check (char ‘*filename’, char ‘*hdu’, gal_data_t ‘*input’, struct gal_tile_two_layer_params ‘*tl’) Make sure that the input parameters (in ‘tl’, short for two-layer) correspond to the input dataset. ‘filename’ and ‘hdu’ are only required for error messages. Also, allocate and fill the ‘tl->channelsize’ array. -- Function: void gal_tile_full_two_layers (gal_data_t ‘*input’, struct gal_tile_two_layer_params ‘*tl’) Create the two layered tessellation in ‘tl’. The general set of steps you need to take to define the two-layered tessellation over an image can be seen in the example code below. gal_data_t *input; struct gal_tile_two_layer_params tl; char *filename="input.fits", *hdu="1"; /* Set all the inputs shown in the structure definition. */ ... /* Read the input dataset. */ input=gal_fits_img_read(filename, hdu, -1, 0, 0); /* Do a sanity check and preparations. */ gal_tile_full_sanity_check(filename, hdu, input, &tl); /* Build the two-layer tessellation*/ gal_tile_full_two_layers(input, &tl); /* `tl.tiles' and `tl.channels' are now a lists of tiles.*/ -- Function: void gal_tile_full_permutation (struct gal_tile_two_layer_params ‘*tl’) Make a permutation to allow the conversion of tile location in memory to its location in the full input dataset and put it in ‘tl->permutation’. If a permutation has already been defined for the tessellation, this function will not do anything. If permutation won’t be necessary (there is only one channel or one dimension), then this function will not do anything (‘tl->permutation’ must have been initialized to ‘NULL’). When there is only one channel OR one dimension, the tiles are allocated in memory in the same order that they represent the input data. However, to make channel-independent processing possible in a generic way, the tiles of each channel are allocated contiguously. So, when there is more than one channel AND more than one dimension, the index of the tile does not correspond to its position in the grid covering the input dataset. The example below may help clarify: assume you have a 6x6 tessellation with two channels in the horizontal and one in the vertical. On the left you can see how the tile IDs correspond to the input dataset. NOTE how ‘03’ is on the second row, not on the first after ‘02’. On the right, you can see how the tiles are stored in memory (and shown if you simply write the array into a FITS file for example). Corresponding to input In memory ---------------------- -------------- 15 16 17 33 34 35 30 31 32 33 34 35 12 13 14 30 31 32 24 25 26 27 28 29 09 10 11 27 28 29 18 19 20 21 22 23 06 07 08 24 25 26 <-- 12 13 14 15 16 17 03 04 05 21 22 23 06 07 08 09 10 11 00 01 02 18 19 20 00 01 02 03 04 05 As a result, if your values are stored in same order as the tiles, and you want them in over-all memory (for example to save as a FITS file), you need to permute the values: gal_permutation_apply(values, tl->permutation); If you have values over-all and you want them in tile-order, you can apply the inverse permutation: gal_permutation_apply_inverse(values, tl->permutation); Recall that this is the definition of permutation in this context: permute: IN_ALL[ i ] = IN_MEMORY[ perm[i] ] inverse: IN_ALL[ perm[i] ] = IN_MEMORY[ i ] -- Function: void gal_tile_full_values_write (gal_data_t ‘*tilevalues’, struct gal_tile_two_layer_params ‘*tl’, int ‘withblank’, char ‘*filename’, gal_fits_list_key_t ‘*keys’, char ‘*program_string’) Write one value for each tile into a file. It is important to note that the values in ‘tilevalues’ must be ordered in the same manner as the tiles, so ‘tilevalues->array[i]’ is the value that should be given to ‘tl->tiles[i]’. The ‘tl->permutation’ array must have been initialized before calling this function with ‘gal_tile_full_permutation’. If ‘withblank’ is non-zero, then block structure of the tiles will be checked and all blank pixels in the block will be blank in the final output file also. -- Function: gal_data_t * gal_tile_full_values_smooth (gal_data_t ‘*tilevalues’, struct gal_tile_two_layer_params ‘*tl’, size_t ‘width’, size_t ‘numthreads’) Smooth the given values with a flat kernel of the given ‘width’. This cannot be done manually because if ‘tl->workoverch==0’, tiles in different channels must not be mixed/smoothed. Also the tiles are contiguous within the channel, not within the image, see the description under ‘gal_tile_full_permutation’. -- Function: size_t gal_tile_full_id_from_coord (struct gal_tile_two_layer_params ‘*tl’, size_t ‘*coord’) Return the ID of the tile that corresponds to the coordinates ‘coord’. Having this ID, you can use the ‘tl->tiles’ array to get to the proper tile or read/write a value into an array that has one value per tile. -- Function: void gal_tile_full_free_contents (struct gal_tile_two_layer_params ‘*tl’) Free all the allocated arrays within ‘tl’.  File: gnuastro.info, Node: Bounding box, Next: Polygons, Prev: Tessellation library, Up: Gnuastro library 10.3.14 Bounding box (‘box.h’) ------------------------------ Functions related to reporting a the bounding box of certain inputs are declared in ‘gnuastro/box.h’. All coordinates in this header are in the FITS format (first axis is the horizontal and the second axis is vertical). -- Function: void gal_box_bound_ellipse_extent (double ‘a’, double ‘b’, double ‘theta_deg’, double ‘*extent’) Return the maximum extent along each dimension of the given ellipse from the center of the ellipse. Therefore this is half the extent of the box in each dimension. ‘a’ is the ellipse major axis, ‘b’ is the minor axis, ‘theta_deg’ is the position angle in degrees. The extent in each dimension is in floating point format and stored in ‘extent’ which must already be allocated before this function. -- Function: void gal_box_bound_ellipse (double ‘a’, double ‘b’, double ‘theta_deg’, long ‘*width’) Any ellipse can be enclosed into a rectangular box. The purpose of this function is to give the height and width of that box assuming the center of the ellipse is in the box center. ‘a’ is the ellipse major axis, ‘b’ is the minor axis, ‘theta_deg’ is the position angle in degrees. The ‘width’ array will contain the output size in long integer type. ‘width[0]’, and ‘width[1]’ are the number of pixels along the first and second FITS axis. Since the ellipse center is assumed to be in the center of the box, all the values in ‘width’ will be an odd integer. -- Function: void gal_box_border_from_center (double ‘center’, size_t ‘ndim’, long ‘*width’, long ‘*fpixel’, long ‘*lpixel’) Given the center coordinates in ‘center’ and the ‘width’ (along each dimension) of a box, return the coordinates of the first (‘fpixel’) and last (‘lpixel’) pixels. All arrays must have ‘ndim’ elements (one for each dimension). -- Function: int gal_box_overlap (long ‘*naxes’, long ‘*fpixel_i’, long ‘*lpixel_i’, long ‘*fpixel_o’, long ‘*lpixel_o’, size_t ‘ndim’) An ‘ndim’-dimensional dataset of size ‘naxes’ (along each dimension, in FITS order) and a box with first and last (inclusive) coordinate of ‘fpixel_i’ and ‘lpixel_i’ is given. This box doesn’t necessarily have to lie within the dataset, it can be outside of it, or only patially overlap. This function will change the values of ‘fpixel_i’ and ‘lpixel_i’ to exactly cover the overlap in the input dataset’s coordinates. This function will return 1 if there is an overlap and 0 if there isn’t. When there is an overlap, the coordinates of the first and last pixels of the overlap will be put in ‘fpixel_o’ and ‘lpixel_o’.  File: gnuastro.info, Node: Polygons, Next: Qsort functions, Prev: Bounding box, Up: Gnuastro library 10.3.15 Polygons (‘polygon.h’) ------------------------------ Polygons are commonly necessary in image processing. In Gnuastro, they are used in Crop (see *note Crop::) for cutting out non-rectangular regions of a image. Warp (see *note Warp::) uses them to warp the images into a new pixel grid. The polygon related Gnuastro library macros and functions are introduced here. In all the functions here the vertices (and points) are defined as an array. So a polygon with 4 vertices will be identified with an array of 8 elements with the first two elements keeping the 2D coordinates of the first vertice and so on. -- Macro: GAL_POLYGON_MAX_CORNERS The largest number of vertices a polygon can have in this library. -- Macro: GAL_POLYGON_ROUND_ERR We have to consider floating point round-off errors when dealing with polygons. For example we will take ‘A’ as the maximum of ‘A’ and ‘B’ when ‘A>B-GAL_POLYGON_ROUND_ERR’. -- Function: void gal_polygon_ordered_corners (double ‘*in’, size_t ‘n’, size_t ‘*ordinds’) We have a simple polygon (that can result from projection, so its edges don’t collide or it doesn’t have holes) and we want to order its corners in an anticlockwise fashion. This is necessary for clipping it and finding its area later. The input vertices can have practically any order. The input (‘in’) is an array containing the coordinates (two values) of each vertice. ‘n’ is the number of corners. So ‘in’ should have ‘2*n’ elements. The output (‘ordinds’) is an array with ‘n’ elements specifying the indexs in order. This array must have been allocated before calling this function. The indexes are output for more generic usage, for example in a homographic transform (necessary in warping an image, see *note Warping basics::), the necessary order of vertices is the same for all the pixels. In other words, only the positions of the vertices change, not the way they need to be ordered. Therefore, this function would only be necessary once. As a summary, the input is unchanged, only ‘n’ values will be put in the ‘ordinds’ array. Such that calling the input coordinates in the following fashion will give an anti-clockwise order when there are 4 vertices: 1st vertice: in[ordinds[0]*2], in[ordinds[0]*2+1] 2nd vertice: in[ordinds[1]*2], in[ordinds[1]*2+1] 3rd vertice: in[ordinds[2]*2], in[ordinds[2]*2+1] 4th vertice: in[ordinds[3]*2], in[ordinds[3]*2+1] The implementation of this is very similar to the Graham scan in finding the Convex Hull. However, in projection we will never have a concave polygon (the left condition below, where this algorithm will get to E before D), we will always have a convex polygon (right case) or E won’t exist! Concave Polygon Convex Polygon D --------C D------------- C \ | E / | \E | \ | / | \ | A--------B A ----------B This is because we are always going to be calculating the area of the overlap between a quadrilateral and the pixel grid or the quadrilateral its self. The ‘GAL_POLYGON_MAX_CORNERS’ macro is defined so there will be no need to allocate these temporary arrays separately. Since we are dealing with pixels, the polygon can’t really have too many vertices. -- Function: double gal_polygon_area (double ‘*v’, size_t ‘n’) Find the area of a polygon with vertices defined in ‘v’. ‘v’ points to an array of doubles which keep the positions of the vertices such that ‘v[0]’ and ‘v[1]’ are the positions of the first vertice to be considered. -- Function: int gal_polygon_pin (double ‘*v’, double ‘*p’, size_t ‘n’) Return ‘1’ if the point ‘p’ is within the polygon whose vertices are defined by ‘v’ and ‘0’ otherwise. Note that the vertices of the polygon have to be sorted in an anti-clock-wise manner. -- Function: int gal_polygon_ppropin (double ‘*v’, double ‘*p’, size_t ‘n’) Similar to ‘gal_polygon_pin’, except that if the point ‘p’ is on one of the edges of a polygon, this will return ‘0’. -- Function: void gal_polygon_clip (double ‘*s’, size_t ‘n’, double ‘*c’, size_t ‘m’, double ‘*o’, size_t ‘*numcrn’) Clip (find the overlap of) two polygons. This function uses the Sutherland-Hodgman (https://en.wikipedia.org/wiki/Sutherland%E2%80%93Hodgman_algorithm) polygon clipping algorithm. Note that the vertices of both polygons have to be sorted in an anti-clock-wise manner.  File: gnuastro.info, Node: Qsort functions, Next: Permutations, Prev: Polygons, Up: Gnuastro library 10.3.16 Qsort functions (‘qsort.h’) ----------------------------------- The C programming language comes with the ‘qsort’ (Quick sort) function. ‘qsort’ is a generic function which allows you to sort any kind of data structure (not just a single number). To define greater and smaller (for sorting), ‘qsort’ needs another function, even for simple numerical types. To facilitate numerical sorting for Gnuastro’s programs/libraries, Gnuastro defines a function for each type’s increasing and decreasing function. You can pass these functions to ‘qsort’ when your array has the respective type (see *note Numeric data types::). -- Global variable: gal_qsort_index_arr Pointer to a floating point array (‘float *’) to use as a reference in ‘gal_qsort_index_float_decreasing’, see the explanation there for more. -- Function: int gal_qsort_index_float_decreasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort a ‘size_t’ array based on decreasing values in the ‘gal_qsort_index_arr’ single precision floating point array. The floating point array will not be changed, it is only read. For example, if we have the following source code: #include #include /* qsort is defined in stdlib.h. */ #include int main (void) { size_t s[4]={0, 1, 2, 3}; float f[4]={1.3,0.2,1.8,0.1}; gal_qsort_index_arr=f; qsort(s, 4, sizeof(size_t), gal_qsort_index_float_decreasing); printf("%zu, %zu, %zu, %zu\n", s[0], s[1], s[2], s[3]); return EXIT_SUCCESS; } The output will be: ‘2, 0, 1, 3’. -- Function: int gal_qsort_TYPE_increasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort an ‘TYPE’ array in increasing order (first element will be the smallest). Please replace ‘TYPE’ (in the function name) with one of the *note Numeric data types::, for example ‘gal_qsort_int32_increasing’, or ‘gal_qsort_float64_increasing’. -- Function: int gal_qsort_TYPE_decreasing (const void ‘*a’, const void ‘*b’) When passed to ‘qsort’, this function will sort an ‘TYPE’ array in decreasing order (first element will be the largest). Please replace ‘TYPE’ (in the function name) with one of the *note Numeric data types::, for example ‘gal_qsort_int32_decreasing’, or ‘gal_qsort_float64_decreasing’.  File: gnuastro.info, Node: Permutations, Next: Matching, Prev: Qsort functions, Up: Gnuastro library 10.3.17 Permutations (‘permutation.h’) -------------------------------------- Permutation is the technical name for re-ordering of values. The need for permutations occurs a lot during (mainly low-level) processing. To do permutation, you must provide two inputs: an array of values (that you want to re-order in place) and a permutation array which contains the new index of each element (let’s call it ‘perm’). The diagram below shows the input array before and after the re-ordering. permute: AFTER[ i ] = BEFORE[ perm[i] ] i = 0 .. N-1 inverse: AFTER[ perm[i] ] = BEFORE[ i ] i = 0 .. N-1 The functions here are a re-implementation of the GNU Scientific Library’s ‘gsl_permute’ function. The reason we didn’t use that function was that it uses system-specific types (like ‘long’ and ‘int’) which can have different widths on different systems, hence are not easily convertible to Gnuastro’s fixed width types (see *note Numeric data types::). There is also a separate function for each type, heavily using macros to allow a ‘base’ function to work on all the types. Thus it is hard to read/understand. Hence, Gnuastro contains a re-write of their steps in a new type-agnostic method which is a single function that can work on any type. As described in GSL’s source code and manual, this implementation comes from Donald Knuth’s _Art of computer programming_ book, in the "Sorting and Searching" chapter of Volume 3 (3rd ed). Exercise 10 of Section 5.2 defines the problem and in the answers, Knuth describes the solution. So if you are interested, please have a look there for more. We are in contact with the GSL developers and in the future(1) we will submit these implementations to GSL. If they are finally incorporated there, we will delete this section in future versions. -- Function: void gal_permutation_check (size_t ‘*permutation’, size_t ‘size’) Print how ‘permutation’ will re-order an array that has ‘size’ elements for each element in one one line. -- Function: void gal_permutation_apply (gal_data_t ‘*input’, size_t ‘*permutation’) Apply ‘permutation’ on the ‘input’ dataset (can have any type), see above for the definition of permutation. -- Function: void gal_permutation_apply_inverse (gal_data_t ‘*input’, size_t ‘*permutation’) Apply the inverse of ‘permutation’ on the ‘input’ dataset (can have any type), see above for the definition of permutation. ---------- Footnotes ---------- (1) Gnuastro’s Task 14497 (http://savannah.gnu.org/task/?14497). If this task is still “postponed†when you are reading this and you are interested to help, your help would be very welcome. Both Gnuastro and GSL developers are very busy, hence both would appreciate your help.  File: gnuastro.info, Node: Matching, Next: Statistical operations, Prev: Permutations, Up: Gnuastro library 10.3.18 Matching (‘match.h’) ---------------------------- Matching is often necessary when the measurements have been done using different instruments, different software or different configurations of the same software. The functions in this part of Gnuastro’s library will be growing to allow matching of images and finding a match between different catalogs (register them). Currently it only provides the The high-level measurements are stored in tables with positions (commonly in RA and Dec with units of degrees). -- Function: gal_data_t * gal_match_coordinates (gal_data_t ‘*coord1’, gal_data_t ‘*coord2’, double ‘*aperture’, int ‘sorted_by_first’, int ‘inplace’, size_t ‘minmapsize’, size_t ‘*nummatched’) Return the permutations that when applied, the first ‘nummatched’ rows of both inputs match with each other (are the nearest within the given aperture). The two inputs (‘coord1’ and ‘coord2’) must be *note List of gal_data_t::. Each ‘gal_data_t’ node in the list should be a single dimensional dataset (column in a table). The dimensions of the coordinates is determined by the number of ‘gal_data_t’ nodes in the two input lists (which must be equal). Note that the number of rows (or the number of elements in each ‘gal_data_t’) in the columns of ‘coord1’ and ‘coord2’ can be different. The matching aperture is defined by the ‘aperture’ array. If several points of one catalog lie within this aperture of a point in the other, the nearest is defined as the match. In a 2D situation (where the input lists have two nodes), for the most generic case, it must have three elements: the major axis length, axis ratio and position angle (see *note Defining an ellipse::). If ‘aperture[1]==1’, the aperture will be a circle of radius ‘aperture[0]’ and the third value won’t be used. When the aperture is an ellipse, distances between the points are also calculated in the respective elliptical distances ($r_{el}$ in *note Defining an ellipse::). To speed up the search, this function will sort the input coordinates by their first column (first axis). If _both_ are already sorted by their first column, you can avoid the sorting step by giving a non-zero value to ‘sorted_by_first’. When sorting is necessary and ‘inplace’ is non-zero, the actual input columns will be sorted. Otherwise, an internal copy of the inputs will be made, used (sorted) and later freed before returning. Therefore, when ‘inplace==0’, inputs will remain untouched, but this function will take more time and memory. If internal allocation is necessary and the space is larger than ‘minmapsize’, the space will be not allocated in the RAM, but in a file, see description of ‘--minmapsize’ in *note Processing options::. The number of matches will be put in the space pointed by ‘nummatched’. If there wasn’t any match, this function will return ‘NULL’. If match(s) were found, a list with three ‘gal_data_t’ nodes will be returned. The top two nodes in the list are the permutations that must be applied to the first and second inputs respectively. After applying the permutations, the top ‘nummatched’ elements will match with each other. The third node is the distances between the respective match. Note that the three nodes of the list are all one-dimensional (a column) and can have different lengths. *Output permutations ignore internal sorting*: the output permutations will correspond to the initial inputs. Therefore, even when ‘inplace!=0’ (and this function re-arranges the inputs), the output permutation will correspond to original (possibly non-sorted) inputs. The reason for this is that you rarely want the actual positional columns after the match. Usually, you also have other columns (measurements, for example magnitudes) for higher-level processing after the match (that correspond to the input order before sorting). Once you have the permutations, they can be applied to those other columns (see *note Permutations::) and the higher-level processing can continue. When you read the coordinates from a table using ‘gal_table_read’ (see *note Table input output::), and only ask for the coordinate columns, the inputs to this function are the returned ‘gal_data_t *’ from two different tables.  File: gnuastro.info, Node: Statistical operations, Next: Binary datasets, Prev: Matching, Up: Gnuastro library 10.3.19 Statistical operations (‘statistics.h’) ----------------------------------------------- After reading a dataset into memory from a file or fully simulating it with another process, the most common processes that will be done on it are statistical operations to let you quantify different aspects of the data. the functions in this section describe Gnuastro’s current set of tools for this job. All these functions can work on any numeric data type natively (see *note Numeric data types::) and can also work on tiles over a dataset. Hence the inputs and outputs are in Gnuastro’s *note Generic data container::. -- Macro: GAL_STATISTICS_SIG_CLIP_MAX_CONVERGE The maximum number of clips, when $\sigma$-clipping should be done by convergence. If the clipping does not converge before making this many clips, all sigma-clipping outputs will be NaN. -- Macro: GAL_STATISTICS_MODE_GOOD_SYM The minimum acceptable symmetricity of the mode calculation. If the symmetricity of the derived mode is less than this value, all the returned values by ‘gal_statistics_mode’ will have a value of NaN. -- Macro: GAL_STATISTICS_SORTED_NOT -- Macro: GAL_STATISTICS_SORTED_INCREASING -- Macro: GAL_STATISTICS_SORTED_DECREASING Macros used to identify if the dataset is sorted and increasing, sorted and decreasing or not sorted. -- Macro: GAL_STATISTICS_BINS_INVALID -- Macro: GAL_STATISTICS_BINS_REGULAR -- Macro: GAL_STATISTICS_BINS_IRREGULAR Macros used to identify if the regularity of the bins when defining bins. -- Function: gal_data_t * gal_statistics_number (gal_data_t ‘*input’) Return a single-element ‘uint64’ dataset containing the number of non-blank elements in ‘input’. -- Function: gal_data_t * gal_statistics_minimum (gal_data_t ‘*input’) Return a single-element dataset containing the minimum non-blank value in ‘input’. The numerical datatype of the output is the same as ‘input’. -- Function: gal_data_t * gal_statistics_maximum (gal_data_t ‘*input’) Return a single-element dataset containing the maximum non-blank value in ‘input’. The numerical datatype of the output is the same as ‘input’. -- Function: gal_data_t * gal_statistics_sum (gal_data_t ‘*input’) Return a single-element (‘double’ or ‘float64’) dataset containing the sum of the non-blank values in ‘input’. -- Function: gal_data_t * gal_statistics_mean (gal_data_t ‘*input’) Return a single-element (‘double’ or ‘float64’) dataset containing the mean of the non-blank values in ‘input’. -- Function: gal_data_t * gal_statistics_std (gal_data_t ‘*input’) Return a single-element (‘double’ or ‘float64’) dataset containing the standard deviation of the non-blank values in ‘input’. -- Function: gal_data_t * gal_statistics_mean_std (gal_data_t ‘*input’) Return a two-element (‘double’ or ‘float64’) dataset containing the mean and standard deviation of the non-blank values in ‘input’. The first element of the returned dataset is the mean and the second is the standard deviation. This function will calculate both values in one pass over the dataset. Hence when both the mean and standard deviation of a dataset are necessary, this function is much more efficient than calling ‘gal_statistics_mean’ and ‘gal_statistics_std’ separately. -- Function: gal_data_t * gal_statistics_median (gal_data_t ‘*input’, int ‘inplace’) Return a single-element dataset containing the median of the non-blank values in ‘input’. The numerical datatype of the output is the same as ‘input’. Calculating the median involves sorting the dataset and removing blank values, for better performance (and less memory usage), you can give a non-zero value to the ‘inplace’ argument. In this case, the sorting and removal of blank elements will be done directly on the input dataset. However, after this function the original dataset may have changed (if it wasn’t sorted or had blank values). -- Function: size_t gal_statistics_quantile_index (size_t ‘size’, double ‘quantile’) Return the index of the element that has a quantile of ‘quantile’ assuming the dataset has ‘size’ elements. -- Function: size_t gal_statistics_quantile (gal_data_t ‘*input’, double ‘quantile’, int ‘inplace’) Return a single-element dataset containing the value with in a quantile ‘quantile’ of the non-blank values in ‘input’. The numerical datatype of the output is the same as ‘input’. See ‘gal_statistics_median’ for a description of ‘inplace’. -- Function: size_t gal_statistics_quantile_function_index (gal_data_t ‘*input’, gal_data_t ‘*value’, int ‘inplace’) Return the index of the quantile function (inverse quantile) of ‘input’ at ‘value’. In other words, this function will return the index of the nearest element (of a sorted and non-blank) ‘input’ to ‘value’. See ‘gal_statistics_median’ for a description of ‘inplace’. -- Function: gal_data_t * gal_statistics_quantile_function (gal_data_t ‘*input’, gal_data_t ‘*value’, int ‘inplace’) Return a single-element (‘double’ or ‘float64’) dataset containing the quantile function of the non-blank values in ‘input’ at ‘value’. In other words, this function will return the quantile of ‘value’ in ‘input’. See ‘gal_statistics_median’ for a description of ‘inplace’. -- Function: gal_data_t * gal_statistics_mode (gal_data_t ‘*input’, float ‘mirrordist’, int ‘inplace’) Return a four-element (‘double’ or ‘float64’) dataset that contains the mode of the ‘input’ distribution. This function implements the non-parametric algorithm to find the mode that is described in Appendix C of Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664). In short it compares the actual distribution and its “mirror distribution†to find the mode. In order to be efficient, you can determine how far the comparison goes away from the mirror through the ‘mirrordist’ parameter (think of it as a multiple of sigma/error). See ‘gal_statistics_median’ for a description of ‘inplace’. The output array has the following elements (in the given order, note that counting in C starts from 0). array[0]: mode array[1]: mode quantile. array[2]: symmetricity. array[3]: value at the end of symmetricity. -- Function: gal_data_t * gal_statistics_mode_mirror_plots (gal_data_t ‘*input’, gal_data_t ‘*value’, size_t ‘numbins’, int ‘inplace’, double ‘*mirror_val’) Make a mirrored histogram and cumulative frequency plot (with ‘numbins’) with the mirror distribution of the ‘input’ with a value at ‘value’. The output is a list of data structures (see *note List of gal_data_t::): the first is the bins with one bin at the mirror point, the second is the histogram with a maximum of one and the third is the cumulative frequency plot (with a maximum of one). -- Function: int gal_statistics_is_sorted (gal_data_t ‘*input’) Return the respective sort macro (see above) for the ‘input’ dataset. -- Function: void gal_statistics_sort_increasing (gal_data_t ‘*input’) Sort the input dataset (in place) in an increasing order. -- Function: void gal_statistics_sort_decreasing (gal_data_t ‘*input’) Sort the input dataset (in place) in a decreasing order. -- Function: gal_data_t * gal_statistics_no_blank_sorted (gal_data_t ‘*input’, int ‘inplace’) Remove all the blanks and sort the input dataset. If ‘inplace’ is non-zero this will happen on the input dataset (and the output will be the same as the input). However, if ‘inplace’ is zero, this function will allocate a new copy of the dataset that is sorted and has no blank values. -- Function: gal_data_t * gal_statistics_regular_bins (gal_data_t ‘*input’, gal_data_t ‘*inrange’, size_t ‘numbins’, double ‘onebinstart’) Generate an array of regularly spaced elements as a 1D array (column) of type ‘double’ (i.e., ‘float64’, it has to be double to account for small differences on the bin edges). The input arguments are described below ‘input’ The dataset you want to apply the bins to. This is only necessary if the range argument is not complete, see below. If ‘inrange’ has all the necessary information, you can pass a ‘NULL’ pointer for this. ‘inrange’ This dataset keeps the desired range along each dimension of the input data structure, it has to be in ‘float’ (i.e., ‘float32’) type. • If you want the full range of the dataset (in any dimensions, then just set ‘inrange’ to ‘NULL’ and the range will be specified from the minimum and maximum value of the dataset (‘input’ cannot be ‘NULL’ in this case). • If there is one element for each dimension in range, then it is viewed as a quantile (Q), and the range will be: ‘Q to 1-Q’. • If there are two elements for each dimension in range, then they are assumed to be your desired minimum and maximum values. When either of the two are NaN, the minimum and maximum will be calculated for it. ‘numbins’ The number of bins: must be larger than 0. ‘onebinstart’ A desired value for onebinstart. Note that with this option, the bins won’t start and end exactly on the given range values, it will be slightly shifted to accommodate this request. -- Function: gal_data_t * gal_statistics_histogram (gal_data_t ‘*input’, gal_data_t ‘*bins’, int ‘normalize’, int ‘maxone’) Make a histogram of all the elements in the given dataset with bin values that are defined in the ‘inbins’ structure (see ‘gal_statistics_regular_bins’). ‘inbins’ is not mandatory, if you pass a ‘NULL’ pointer, the bins structure will be built within this function based on the ‘numbins’ input. As a result, when you have already defined the bins, ‘numbins’ is not used. -- Function: gal_data_t * gal_statistics_cfp (gal_data_t ‘*input’, gal_data_t ‘*bins’, int ‘normalize’) Make a cumulative frequency plot (CFP) of all the elements in ‘input’ with bin values that are defined in the ‘bins’ structure (see ‘gal_statistics_regular_bins’). The CFP is built from the histogram: in each bin, the value is the sum of all previous bins in the histogram. Thus, if you have already calculated the histogram before calling this function, you can pass it onto this function as the data structure in ‘bins->next’ (see ‘List of gal_data_t’). If ‘bin->next!=NULL’, then it is assumed to be the histogram. If it is ‘NULL’, then the histogram will be calculated internally and freed after the job is finished. When a histogram is given and it is normalized, the CFP will also be normalized (even if the normalized flag is not set here): note that a normalized CFP’s maximum value is 1. -- Function: gal_data_t * gal_statistics_sigma_clip (gal_data_t ‘*input’, float ‘multip’, float ‘param’, int ‘inplace’, int ‘quiet’) Apply $\sigma$-clipping on a given dataset and return a dataset that contains the results. For a description of $\sigma$-clipping see *note Sigma clipping::. ‘multip’ is the multiple of the standard deviation ($\sigma$ that is used to define outliers in each round of clipping). The role of ‘param’ is determined based on its value. If ‘param’ is larger than ‘1’ (one), it must be an integer and will be interpretted as the number clips to do. If it is less than ‘1’ (one), it is interpretted as the tolerance level to stop the iteration. The output dataset has the following elements with a ‘GAL_TYPE_FLOAT32’ type: array[0]: Number of points used. array[1]: Median. array[2]: Mean. array[3]: Standard deviation.  File: gnuastro.info, Node: Binary datasets, Next: Convolution functions, Prev: Statistical operations, Up: Gnuastro library 10.3.20 Binary datasets (‘binary.h’) ------------------------------------ Binary datasets only have two (usable) values: 0 (also known as background) or 1 (also known as foreground). They are created after some binary classification is applied to the dataset. The most common is thresholding: for example in an image, pixels with a value above the threshold are given a value of 1 and those with a value less than the threshold are assigned a value of 0. Since there is only two values, in the processing of binary images, you are usually concerned with the positioning of an element and its vicinity (neighbors). When a dataset has more than one dimension, multiple classes of immediate neighbors (that are touching the element) can be defined for each data-element. To separate these different classes of immediate neighbors, we define _connectivity_. The classification is done by the distance from element center to the neighbor’s center. The nearest immediate neighbors have a connectivity of 1, the second nearest class of neighbors have a connectivity of 2 and so on. In total, the largest possible connectivity for data with ‘ndim’ dimensions is ‘ndim’. For example in a 2D dataset, 4-connected neighbors (that share an edge and have a distance of 1 pixel) have a connectivity of 1. The other 4 neighbors that only share a vertice (with a distance of $\sqrt{2}$ pixels) have a connectivity of 2. Conventionally, the class of connectivity-2 neighbors also includes the connectivity 1 neighbors, so for example we call them 8-connected neighbors in 2D datasets. Ideally, one bit is sufficient for each element of a binary dataset. However, CPUs are not designed to work on individual bits, the smallest unit of memory addresses is a byte (containing 8 bits on modern CPUs). Therefore, in Gnuastro, the type used for binary dataset is ‘uint8_t’ (see *note Numeric data types::). Although it does take 8-times more memory, this choice offers much better performance and the some extra (useful) features. The advantage of using a full byte for each element of a binary dataset is that you can also have other values (that will be ignored in the processing). One such common “other†value in real datasets is a blank value (to mark regions that should not be processed because there is no data). The constant ‘GAL_BLANK_UINT8’ value must be used in these cases (see *note Library blank values::). Another is some temporary value(s) that can be given to a processed pixel to avoid having another copy of the dataset as in ‘GAL_BINARY_TMP_VALUE’ that is described below. -- Macro: GAL_BINARY_TMP_VALUE The functions described below work on a ‘uint8_t’ type dataset with values of 1 or 0 (no other pixel will be touched). However, in some cases, it is necessary to put temporary values in each element during the processing of the functions. This temporary value has a special meaning for the operation and will be operated on. So if your input datasets have values other than 0 and 1 that you don’t want these functions to work on, be sure they are not equal to this macro’s value. Note that this value is also different from ‘GAL_BLANK_UINT8’, so your input datasets may also contain blank elements. -- Function: gal_data_t * gal_binary_erode (gal_data_t ‘*input’, size_t ‘num’, int ‘connectivity’, int ‘inplace’) Do ‘num’ erosions on the ‘connectivity’-connected neighbors of ‘input’ (see above for the definition of connectivity). If ‘inplace’ is non-zero _and_ the input’s type is ‘GAL_TYPE_UINT8’, then the erosion will be done within the input dataset and the returned pointer will be ‘input’. Otherwise, ‘input’ is copied (and converted if necessary) to ‘GAL_TYPE_UINT8’ and erosion will be done on this new dataset which will also be returned. This function will only work on the elements with a value of 1 or 0. It will leave all the rest unchanged. Erosion (inverse of dilation) is an operation in mathematical morphology where each foreground pixel that is touching a background pixel is flipped (changed to background). The ‘connectivity’ value determines the definition of “touchingâ€. Erosion will thus decrease the area of the foreground regions by one layer of pixels. -- Function: gal_data_t * gal_binary_dilate (gal_data_t ‘*input’, size_t ‘num’, int ‘connectivity’, int ‘inplace’) Do ‘num’ dilations on the ‘connectivity’-connected neighbors of ‘input’ (see above for the definition of connectivity). For more on ‘inplace’ and the output, see ‘gal_binary_erode’. Dilation (inverse of erosion) is an operation in mathematical morphology where each background pixel that is touching a foreground pixel is flipped (changed to foreground). The ‘connectivity’ value determines the definition of “touchingâ€. Dilation will thus increase the area of the foreground regions by one layer of pixels. -- Function: gal_data_t * gal_binary_open (gal_data_t ‘*input’, size_t ‘num’, int ‘connectivity’, int ‘inplace’) Do ‘num’ openings on the ‘connectivity’-connected neighbors of ‘input’ (see above for the definition of connectivity). For more on ‘inplace’ and the output, see ‘gal_binary_erode’. Opening is an operation in mathematical morphology which is defined as erosion followed by dilation (see above for the definitions of erosion and dilation). Opening will thus remove the outer structure of the foreground. In this implementation, ‘num’ erosions are going to be applied on the dataset, then ‘num’ dilations. -- Function: size_t gal_binary_connected_components (gal_data_t ‘*binary’, gal_data_t ‘**out’, int ‘connectivity’) Return the number of connected components in ‘binary’ through the breadth first search algorithm (finding all pixels belonging to one component before going on to the next). Connection between two pixels is defined based on the value to ‘connectivity’. ‘out’ is a dataset with the same size as ‘binary’ with ‘GAL_TYPE_INT32’ type. Every pixel in ‘out’ will have the label of the connected component it belongs to. The labeling of connected components starts from 1, so a label of zero is given to the input’s background pixels. When ‘*out!=NULL’ (its space is already allocated), it will be cleared (to zero) at the start of this function. Otherwise, when ‘*out==NULL’, the necessary dataset to keep the output will be allocated by this function. ‘binary’ must have a type of ‘GAL_TYPE_UINT8’, otherwise this function will abort with an error. Other than blank pixels (with a value of ‘GAL_BLANK_UINT8’ defined in *note Library blank values::), all other non-zero pixels in ‘binary’ will be considered as foreground (and will be labeled). Blank pixels in the input will also be blank in the output. -- Function: gal_data_t * gal_binary_connected_adjacency_matrix (gal_data_t ‘*adjacency’, size_t ‘*numconnected’) Find the number of connected labels and new labels based on an adjacency matrix, which must be a square binary array (type ‘GAL_TYPE_UINT8’). The returned dataset is a list of new labels for each old label. In other words, this function will find the objects that are connected (possibly through a third object) and in the output array, the respective elements for all input labels is going to have the same value. The total number of connected labels is put into the space that ‘numconnected’ points to. An adjacency matrix defines connection between two labels. For example, let’s assume we have 5 labels and we know that labels 1 and 5 are connected to label 3, but are not connected with each other. Also, labels 2 and 4 are not touching any other label. So in total we have 3 final labels: one combined object (merged from labels 1, 3, and 5) and the initial labels 2 and 4. The input adjacency matrix would look like this (note the extra row and column for a label 0 which is ignored): INPUT OUTPUT ===== ====== in_lab 1 2 3 4 5 | | numconnected = 3 0 0 0 0 0 0 | in_lab 1 --> 0 0 0 1 0 0 | in_lab 2 --> 0 0 0 0 0 0 | Returned: new labels for the in_lab 3 --> 0 1 0 0 0 1 | 5 initial objects in_lab 4 --> 0 0 0 0 0 0 | | 0 | 1 | 2 | 1 | 3 | 1 | in_lab 5 --> 0 0 0 1 0 0 | Although the adjacency matrix as used here is symmetric, currently this function assumes that it is filled on both sides of the diagonal. -- Function: void gal_binary_fill_holes (gal_data_t ‘*input’, int ‘connectivity’) Fill all the holes (0 valued pixels surrounded by 1 valued pixels) within a region of the binary ‘input’ dataset. The connectivity of the holes can be set with ‘connectivity’. This function currently only works on a 2D dataset.  File: gnuastro.info, Node: Convolution functions, Next: Interpolation, Prev: Binary datasets, Up: Gnuastro library 10.3.21 Convolution functions (‘convolve.h’) -------------------------------------------- Convolution is a very common operation during data analysis and is thoroughly described as part of Gnuastro’s *note Convolve:: program which is fully devoted to this job. Because of the complete introduction that was presented there, we will directly skip onto the currently available convolution functions in Gnuastro’s library. As of this version, only spatial domain convolution is available in Gnuastro’s libraries. We haven’t had the time to liberate the frequency domain function convolution and de-convolution functions that are available in the Convolve program(1). -- Function: gal_data_t * gal_convolve_spatial (gal_data_t ‘*tiles’, gal_data_t ‘*kernel’, size_t ‘numthreads’, int ‘edgecorrection’, int ‘convoverch’) Convolve each node of the list of ‘tiles’ (see *note List of gal_data_t:: and *note Tessellation library::) with ‘kernel’ using ‘numthreads’. When ‘edgecorrection’ is non-zero, it will correct for the edge dimming effects as discussed in *note Edges in the spatial domain::. To create a tessellation that fully covers an input image, you may use ‘gal_tile_full’, or ‘gal_tile_full_two_layers’ to also define channels over your input dataset. These functions are discussed in *note Tile grid::. You may then pass the list of tiles to this function. This is the recommended way to call this function because spatial domain convolution is slow and breaking the job into many small tiles and working on simultaneously on several threads can greatly speed up the processing. If the tiles are defined within a channel (a larger tile), by default convolution will be done within the channel, so pixels on the edge of a channel will not be affected by their neighbors that are in another channel. See *note Tessellation:: for the necessity of channels in astronomical data analysis. This behavior may be disabled when ‘convoverch’ is non-zero. In this case, it will ignore channel borders (if they exist) and mix all pixels that cover the kernel within the dataset. -- Function: void gal_convolve_spatial_correct_ch_edge (gal_data_t ‘*tiles’, gal_data_t ‘*kernel’, size_t ‘numthreads’, int ‘edgecorrection’, gal_data_t ‘*tocorrect’) Correct the edges of channels in an already convolved image when it was initially convolved with ‘gal_convolve_spatial’ and ‘convoverch==0’. In that case, strong boundaries might exist on the channel edges. So if you later need to remove those boundaries at later steps of your processing, you can call this function. It will only do convolution on the tiles that are near the edge and were effected by the channel borders. Other pixels in the image will not be touched. Hence, it is much faster. ---------- Footnotes ---------- (1) Hence any help would be greatly appreciated.  File: gnuastro.info, Node: Interpolation, Next: Git wrappers, Prev: Convolution functions, Up: Gnuastro library 10.3.22 Interpolation (‘interpolate.h’) --------------------------------------- During data analysis, it often happens that parts of the data cannot be given a value. For example your image was saturated due to a very bright start and you have to mask that star’s footprint. One other common situation in Gnuastro is when we do processing on tiles (for example to estimate the Sky value and its Standard deviation, see *note Sky value::). Some tiles must not be used for the estimation of the Sky value, for example because they cover a large galaxy. So we need to fill them in with blank values. But ultimately, we need a Sky value for every pixel. This job (assigning a value to blank element(s) based on their nearby neighbors with a value) is known as interpolation. There are many ways to do interpolation, but (mainly due to lack of time), currently Gnuastro only contains the (median of) nearest-neighbor method. The power of this method of interpolation is its non-parametric nature. The produced values are also always within the range of the known values and strong outliers do not get created. We will hopefully implement other methods too (wrappers around the GNU Scientific Library’s very complete set of functions), but currently the developers are too busy. So if you do have the chance to help your contribution would be very welcome and appreciated. -- Function: gal_data_t * gal_interpolate_close_neighbors (gal_data_t ‘*input’, struct gal_tile_two_layer_params ‘*tl’, size_t ‘numneighbors’, size_t ‘numthreads’, int ‘onlyblank’, int ‘aslinkedlist’) Interpolate the values in the image using the median value of their ‘numneighbors’ closest neighbors. If ‘onlyblank’ is non-zero, then only blank elements will be interpolated and pixels that already have a value will be left untouched. This function is multi-threaded and will run on ‘numthreads’ threads (see ‘gal_threads_number’ in *note Multithreaded programming::). ‘tl’ is Gnuastro’s two later tessellation structure used to define tiles over an image and is fully described in *note Tile grid::. When ‘tl!=NULL’, then it is assumed that the ‘input->array’ contains one value per tile and interpolation will respect certain tessellation properties, for example to not interpolate over channel borders. If several datasets have the same set of blank values, you don’t need to call this function multiple times. When ‘aslinkedlist’ is non-zero, then ‘input’ will be seen as a *note List of gal_data_t:: and for all the same neighbor position checking will be done for all the datasets in the list. Of course, the values for each dataset will be different, so a different value will be written in the each dataset, but the neighbor checking that is the most CPU intensive part will only be done once.  File: gnuastro.info, Node: Git wrappers, Next: Cosmology library, Prev: Interpolation, Up: Gnuastro library 10.3.23 Git wrappers (‘git.h’) ------------------------------ Git is one of the most common tools for version control and it can often be useful during development, for example see ‘COMMIT’ keyword in *note Output headers::. At installation time, Gnuastro will also check for the existence of libgit2, and store the value in the ‘GAL_CONFIG_HAVE_LIBGIT2’, see *note Configuration information:: and *note Optional dependencies::. ‘gnuastro/git.h’ includes ‘gnuastro/config.h’ internally, so you won’t have to include both for this macro. -- Function: char * gal_git_describe ( ) When libgit2 is present and the program is called within a directory that is version controlled, this function will return a string containing the commit description (similar to Gnuastro’s unofficial version number, see *note Version numbering::). If there are uncommitted changes in the running directory, it will add a ‘‘-dirty’’ prefix to the description. When there is no tagged point in the previous commit, this function will return a uniquely abbreviated commit object as fallback. This function is used for generating the value of the ‘COMMIT’ keyword in *note Output headers::. The output string is similar to the output of the following command: $ git describe --dirty --always Space for the output string is allocated within this function, so after using the value you have to ‘free’ the output string. If libgit2 is not installed or the program calling this function is not within a version controlled directory, then the output will be the ‘NULL’ pointer.  File: gnuastro.info, Node: Cosmology library, Prev: Git wrappers, Up: Gnuastro library 10.3.24 Cosmology library (‘cosmology.h’) ----------------------------------------- This library does the main cosmological calculations that are commonly necessary in extra-galactic astronomical studies. The main variable in this context is the redshift ($z$). The cosmological input parameters in the functions below are ‘H0’, ‘o_lambda_0’, ‘o_matter_0’, ‘o_radiation_0’ which respectively represent the current (at redshift 0) expansion rate (Hubble constant in units of km/sec/Mpc), cosmological constant ($\Lambda$), matter and radiation densities. All these functions are declared in ‘gnuastro/cosmology.h’. For a more extended introduction/discussion of the cosmological parameters, please see *note CosmicCalculator::. -- Function: double gal_cosmology_age (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Returns the age of the universe at redshift ‘z’ in units of Giga years. -- Function: double gal_cosmology_proper_distance (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Returns the proper distance to an object at redshift ‘z’ in units of Mega parsecs. -- Function: double gal_cosmology_comoving_volume (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Returns the comoving volume over 4pi stradian to ‘z’ in units of Mega parsecs cube. -- Function: double gal_cosmology_critical_density (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Returns the critical density at redshift ‘z’ in units of $g/cm^3$. -- Function: double gal_cosmology_angular_distance (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Return the angular diameter distance to an object at redshift ‘z’ in units of Mega parsecs. -- Function: double gal_cosmology_luminosity_distance (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Return the luminosity diameter distance to an object at redshift ‘z’ in units of Mega parsecs. -- Function: double gal_cosmology_distance_modulus (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Return the distance modulus at redshift ‘z’ (with no units). -- Function: double gal_cosmology_to_absolute_mag (double ‘z’, double ‘H0’, double ‘o_lambda_0’, double ‘o_matter_0’, double ‘o_radiation_0’) Return the conversion from apparent to absolute magnitude for an object at redshift ‘z’. This value has to be added to the apparent magnitude to give the absolute magnitude of an object at redshift ‘z’.  File: gnuastro.info, Node: Library demo programs, Prev: Gnuastro library, Up: Library 10.4 Library demo programs ========================== In this final section of *note Library::, we give some example Gnuastro programs to demonstrate various features in the library. All these programs have been tested and once Gnuastro is installed you can compile and run them with with Gnuastro’s *note BuildProgram:: program that will take care of linking issues. If you don’t have any FITS file to experiment on, you can use those that are generated by Gnuastro after ‘make check’ in the ‘tests/’ directory, see *note Quick start::. * Menu: * Library demo - reading a image:: Read a FITS image into memory. * Library demo - inspecting neighbors:: Inspect the neighbors of a pixel. * Library demo - multi-threaded operation:: Doing an operation on threads. * Library demo - reading and writing table columns:: Simple Column I/O.  File: gnuastro.info, Node: Library demo - reading a image, Next: Library demo - inspecting neighbors, Prev: Library demo programs, Up: Library demo programs 10.4.1 Library demo - reading a FITS image ------------------------------------------ The following simple program demonstrates how to read a FITS image into memory and use the ‘void *array’ pointer in of *note Generic data container::. For easy linking/compilation of this program along with a first run see *note BuildProgram::. Before running, also change the ‘filename’ and ‘hdu’ variable values to specify an existing FITS file and/or extension/HDU. This is just intended to demonstrate how to use the ‘array’ pointer of ‘gal_data_t’. Hence it doesn’t do important sanity checks, for example in real datasets you may also have blank pixels. In such cases, this program will return a NaN value (see *note Blank pixels::). So for general statistical information of a dataset, it is much better to use Gnuastro’s *note Statistics:: program which can deal with blank pixels any many other issues in a generic dataset. #include #include #include /* includes gnuastro's data.h and type.h */ #include int main(void) { size_t i; float *farray; double sum=0.0f; gal_data_t *image; char *filename="img.fits", *hdu="1"; /* Read `img.fits' (HDU: 1) as a float32 array. */ image=gal_fits_img_read_to_type(filename, hdu, GAL_TYPE_FLOAT32, -1, 0, 0); /* Use the allocated space as a single precision floating * point array (recall that `image->array' has `void *' * type, so it is not directly usable. */ farray=image->array; /* Calculate the sum of all the values. */ for(i=0; isize; ++i) sum += farray[i]; /* Report the sum. */ printf("Sum of values in %s (hdu %s) is: %f\n", filename, hdu, sum); /* Clean up and return. */ gal_data_free(image); return EXIT_SUCCESS; }  File: gnuastro.info, Node: Library demo - inspecting neighbors, Next: Library demo - multi-threaded operation, Prev: Library demo - reading a image, Up: Library demo programs 10.4.2 Library demo - inspecting neighbors ------------------------------------------ The following simple program shows how you can inspect the neighbors of a pixel using the ‘GAL_DIMENSION_NEIGHBOR_OP’ function-like macro that was introduced in *note Dimensions::. For easy linking/compilation of this program along with a first run see *note BuildProgram::. Before running, also change the file name and HDU (first and second arguments to ‘gal_fits_img_read_to_type’) to specify an existing FITS file and/or extension/HDU. #include #include #include int main(void) { double sum; float *array; size_t i, num, *dinc; gal_data_t *input=gal_fits_img_read_to_type("input.fits", "1", GAL_TYPE_FLOAT32, -1, 0, 0); /* To avoid the `void *' pointer and have `dinc'. */ array=input->array; dinc=gal_dimension_increment(input->ndim, input->dsize); /* Go over all the pixels. */ for(i=0;isize;++i) { num=0; sum=0.0f; GAL_DIMENSION_NEIGHBOR_OP( i, input->ndim, input->dsize, input->ndim, dinc, {++num; sum+=array[nind];} ); printf("%zu: num: %zu, sum: %f\n", i, num, sum); } /* Clean up and return. */ gal_data_free(input); return EXIT_SUCCESS; }  File: gnuastro.info, Node: Library demo - multi-threaded operation, Next: Library demo - reading and writing table columns, Prev: Library demo - inspecting neighbors, Up: Library demo programs 10.4.3 Library demo - multi-threaded operation ---------------------------------------------- The following simple program shows how to use Gnuastro to simplify spinning off threads and distributing different jobs between the threads. The relevant thread-related functions are defined in *note Gnuastro's thread related functions::. For easy linking/compilation of this program, along with a first run, see Gnuastro’s *note BuildProgram::. Before running, also change the ‘filename’ and ‘hdu’ variable values to specify an existing FITS file and/or extension/HDU. This is a very simple program to open a FITS image, distribute its pixels between different threads and print the value of each pixel and the thread it was assigned to. The actual operation is very simple (and would not usually be done with threads in a real-life program). It is intentionally chosen to put more focus on the important steps in spinning of threads and how the worker function (which is called by each thread) can identify the job-IDs it should work on. For example, instead of an array of pixels, you can define an array of tiles or any other context-specific structures as separate targets. The important thing is that each action should have its own unique ID (counting from zero, as is done in an array in C). You can then follow the process below and use each thread to work on all the targets that are assigned to it. Recall that spinning-off threads is its self an expensive process and we don’t want to spin-off one thread for each target (see the description of ‘gal_threads_dist_in_threads’ in *note Gnuastro's thread related functions::. There are many (more complicated, real-world) examples of using ‘gal_threads_spin_off’ in Gnuastro’s actual source code, you can see them by searching for the ‘gal_threads_spin_off’ function from the top source (after unpacking the tarball) directory (for example with this command): $ grep -r gal_threads_spin_off ./ The code of this demonstration program is shown below. This program was also built and run when you ran ‘make check’ during the building of Gnuastro (‘tests/lib/multithread.c’, so it is already tested for your system and you can safely use it as a guide. #include #include #include "gnuastro/fits.h" #include "gnuastro/threads.h" /* This structure can keep all information you want to pass onto the * worker function on each thread. */ struct params { gal_data_t *image; /* Dataset to print values of. */ }; /* This is the main worker function which will be called by the * different threads. `gal_threads_params' is defined in * `gnuastro/threads.h' and contains the pointer to the parameter we * want. Note that the input argument and returned value of this * function always must have `void *' type. */ void * worker_on_thread(void *in_prm) { /* Low-level definitions to be done first. */ struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct params *p=(struct params *)tprm->params; /* Subsequent definitions. */ float *array=p->image->array; size_t i, index, *dsize=p->image->dsize; /* Go over all the actions (pixels in this case) that were assigned * to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* For easy reading. */ index = tprm->indexs[i]; /* Print the information. */ printf("(%zu, %zu) on thread %zu: %g\n", index%dsize[1]+1, index/dsize[1]+1, tprm->id, array[index]); } /* Wait for all the other threads to finish, then return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* High-level function (called by the operating system). */ int main(void) { struct params p; char *filename="input.fits", *hdu="1"; size_t numthreads=gal_threads_number(); /* Read the image into memory as a float32 data type. We are using * `-1' for `minmapsize' to ensure that the image is read into * memory. */ p.image=gal_fits_img_read_to_type(filename, hdu, GAL_TYPE_FLOAT32, -1, 0, 0); /* Print some basic information before the actual contents: */ printf("Pixel values of %s (HDU: %s) on %zu threads.\n", filename, hdu, numthreads); printf("Used to check the compiled library's capability in opening " "a FITS file, and also spinning-off threads.\n"); /* A small sanity check: this is only intended for 2D arrays (to * print the coordinates of each pixel). */ if(p.image->ndim!=2) { fprintf(stderr, "only 2D images are supported."); exit(EXIT_FAILURE); } /* Spin-off the threads and do the processing on each thread. */ gal_threads_spin_off(worker_on_thread, &p, p.image->size, numthreads); /* Clean up and return. */ gal_data_free(p.image); return EXIT_SUCCESS; }  File: gnuastro.info, Node: Library demo - reading and writing table columns, Prev: Library demo - multi-threaded operation, Up: Library demo programs 10.4.4 Library demo - reading and writing table columns ------------------------------------------------------- Tables are some of the most common inputs to, and outputs of programs. This section contains a small program for reading and writing tables using the constructs described in *note Table input output::. For easy linking/compilation of this program, along with a first run, see Gnuastro’s *note BuildProgram::. Before running, also set the following file and column names in the first two lines of ‘main’. The input and output names may be ‘.txt’ and ‘.fits’ tables, ‘gal_table_read’ and ‘gal_table_write’ will be able to write to both formats. For plain text tables see see *note Gnuastro text table format::. This example program reads three columns from a table. The first two columns are selected by their name (‘NAME1’ and ‘NAME2’) and the third is selected by its number: column 10 (counting from 1). Gnuastro’s column selection is discussed in *note Selecting table columns::. The first and second columns can be any type, but this program will convert them to ‘int32_t’ and ‘float’ for its internal usage respectively. However, the third column must be double for this program. So if it isn’t, the program will abort with an error. Having the columns in memory, it will print them out along with their sum (just a simple application, you can do what ever you want at this stage). Reading the table finishes here. The rest of the program is a demonstration of writing a table. While parsing the rows, this program will change the first column (to be counters) and multiply the second by 10 (so the output will be different). Then it will define the order of the output columns by setting the ‘next’ element (to create a *note List of gal_data_t::). Before writing, this function will also set names for the columns (units and comments can be defined in a similar manner). Writing the columns to a file is then done through a simple call to ‘gal_table_write’. The operations that are shown in this example program are not necessary all the time. For example, in many cases, you know the numerical data type of the column before writing your program (see *note Numeric data types::), so type checking and copying to a specific type won’t be necessary. #include #include #include int main(void) { /* File names and column names (which may also be numbers). */ char *c1_name="NAME1", *c2_name="NAME2", *c3_name="10"; char *inname="input.fits", *hdu="1", *outname="out.fits"; /* Internal parameters. */ float *array2; double *array3; int32_t *array1; size_t i, counter=0; gal_data_t *c1, *c2; gal_data_t tmp, *col, *columns; gal_list_str_t *column_ids=NULL; /* Define the columns to read. */ gal_list_str_add(&column_ids, c1_name, 0); gal_list_str_add(&column_ids, c2_name, 0); gal_list_str_add(&column_ids, c3_name, 0); /* The columns were added in reverse, so correct it. */ gal_list_str_reverse(&column_ids); /* Read the desired columns. */ columns = gal_table_read(inname, hdu, column_ids, GAL_TABLE_SEARCH_NAME, 1, -1, NULL); /* Go over the columns, we'll assume that you don't know their type * a-priori, so we'll check */ counter=1; for(col=columns; col!=NULL; col=col->next) switch(counter++) { case 1: /* First column: we want it as int32_t. */ c1=gal_data_copy_to_new_type(col, GAL_TYPE_INT32); array1 = c1->array; break; case 2: /* Second column: we want it as float. */ c2=gal_data_copy_to_new_type(col, GAL_TYPE_FLOAT32); array2 = c2->array; break; case 3: /* Third column: it MUST be double. */ if(col->type!=GAL_TYPE_FLOAT64) { fprintf(stderr, "Column %s must be float64 type, it is " "%s", c3_name, gal_type_name(col->type, 1)); exit(EXIT_FAILURE); } array3 = col->array; break; } /* As an example application we'll just print them out. In the * meantime (just for a simple demonstration), change the first * array value to the counter and multiply the second by 10. */ for(i=0;isize;++i) { printf("%zu: %d + %f + %f = %f\n", i+1, array1[i], array2[i], array3[i], array1[i]+array2[i]+array3[i]); array1[i] = i+1; array2[i] *= 10; } /* Link the first two columns as a list. */ c1->next = c2; c2->next = NULL; /* Set names for the columns and write them out. */ c1->name = "COUNTER"; c2->name = "VALUE"; gal_table_write(c1, NULL, GAL_TABLE_FORMAT_BFITS, outname); /* The names weren't allocated, so to avoid cleaning-up problems, * we'll set them to NULL. */ c1->name = c2->name = NULL; /* Clean up and return. */ gal_data_free(c1); gal_data_free(c2); gal_list_data_free(columns); gal_list_str_free(column_ids, 0); /* strings weren't allocated. */ return EXIT_SUCCESS; }  File: gnuastro.info, Node: Developing, Next: Gnuastro programs list, Prev: Library, Up: Top 11 Developing ************* The basic idea of GNU Astronomy Utilities is for an interested astronomer to be able to easily understand the code of any of the programs or libraries, be able to modify the code if s/he feels there is an improvement and finally, to be able to add new programs or libraries for their own benefit, and the larger community if they are willing to share it. In short, we hope that at least from the software point of view, the “obscurantist faith in the expert’s special skill and in his personal knowledge and authority†can be broken, see *note Science and its tools::. With this aim in mind, Gnuastro was designed to have a very basic, simple, and easy to understand architecture for any interested inquirer. This chapter starts with very general design choices, in particular *note Why C:: and *note Program design philosophy::. It will then get a little more technical about the Gnuastro code and file/directory structure in *note Coding conventions:: and *note Program source::. *note The TEMPLATE program:: discusses a minimal (and working) template to help in creating new programs or easier learning of a program’s internal structure. Some other general issues about documentation, building and debugging are then discussed. This chapter concludes with how you can learn about the development and get involved in *note Gnuastro project webpage::, *note Developing mailing lists:: and *note Contributing to Gnuastro::. * Menu: * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro’s development. * Contributing to Gnuastro:: Share your changes with all users.  File: gnuastro.info, Node: Why C, Next: Program design philosophy, Prev: Developing, Up: Developing 11.1 Why C programming language? ================================ Currently the programming language that is most commonly used in scientific applications is C++(1), Python(2), and Julia(3) (which is a newcomer but swiftly gaining ground). One of the main reasons behind this choice is their high-level abstractions. However, GNU Astronomy Utilities is fully written in the C programming language(4). The reasons can be summarized with simplicity, portability and efficiency/speed. All three are very important in a scientific software and we will discuss them below. Simplicity can best be demonstrated in a comparison of the main books of C++ and C. The “C programming languageâ€(5) book, written by the authors of C, is only 286 pages and covers a very good fraction of the language, it has also remained unchanged from 1988. C is the main programming language of nearly all operating systems and there is no plan of any significant update. On the other hand, the most recent “C++ programming languageâ€(6) book, also written by its author, has 1366 pages and its fourth edition came out in 2013! As discussed in *note Science and its tools::, it is very important for other scientists to be able to readily read the code of a program at their will with minimum requirements. In C++, inheriting objects in the object oriented programming paradigm and their internal functions make the code very easy to write for a programmer who is deeply invested in those objects and understands all their relations well. But it simultaneously makes reading the program for a first time reader (a curious scientist who wants to know only how a small step was done) extremely hard. Before understanding the methods, the scientist has to invest a lot of time and energy in understanding those objects and their relations. But in C, everything is done with basic language types for example ‘int’s or ‘float’s and their pointers to define arrays. So when an outside reader is only interested in one part of the program, that part is all they have to understand. Recently it is also becoming common to write scientific software in Python, or a combination of it with C or C++. Python is a high level scripting language which doesn’t need compilation. It is very useful when you want to do something on the go and don’t want to be halted by the troubles of compiling, linking, memory checking, etc. When the datasets are small and the job is temporary, this ability of Python is great and is highly encouraged. A very good example might be plotting, in which Python is undoubtedly one of the best. But as the data sets increase in size and the processing becomes more complicated, the speed of Python scripts significantly decrease. So when the program doesn’t change too often and is widely used in a large community, mostly on large data sets (like astronomical images), using Python will waste a lot of valuable research-hours. It is possible to wrap C or C++ functions with Python to fix the speed issue. But this creates further complexity, because the interested scientist has to master two programming languages and their connection (which is not trivial). Like C++, Python is object oriented, so as explained above, it needs a high level of experience with that particular program to reasonably understand its inner workings. To make things worse, since it is mainly for on-the-go programming(7), it can undergo significant changes. One recent example is how Python 2.x and Python 3.x are not compatible. Lots of research teams that invested heavily in Python 2.x cannot benefit from Python 3.x or future versions any more. Some converters are available, but since they are automatic, lots of complications might arise in the conversion(8). If a research project begins using Python 3.x today, there is no telling how compatible their investments will be when Python 4.x or 5.x will come out. This stems from the core principles of Python, which are very useful when you look in the ‘on the go’ basis as described before and not future usage. Reproducibility (ability to run the code in the future) is a core principal of any scientific result, or the software that produced that result. Rebuilding all the dependencies of a software in an obsolete language is not easy. Future-proof code (as long as current operating systems will be used) is written in C. The portability of C is best demonstrated by the fact that both C++ and Python are part of the C-family of programming languages which also include Julia, Java, Perl, and many other languages. C libraries can be immediately included in C++, and it is easy to write wrappers for them in all C-family programming languages. This will allow other scientists to benefit from C libraries using any C-family language that they prefer. As a result, Gnuastro’s library is already usable in C and C++, and wrappers will be(9) added for higher-level languages like Python, Julia and Java. The final reason was speed. This is another very important aspect of C which is not independent of simplicity (first reason discussed above). The abstractions provided by the higher-level languages (which also makes learning them harder for a newcomer) comes at the cost of speed. Since C is a low-level language(10) (closer to the hardware), it is much less complex for both the human reader _and_ the computer. The benefits of simplicity for a human were discussed above. Simplicity for the computer translates into more efficiently (faster) programs. This creates a much closer relation between the scientist/programmer (or their program) and the actual data and processing. The GNU coding standards(11) also encourage the use of C over all other languages when generality of usage and “high speed†is desired. ---------- Footnotes ---------- (1) (2) (3) (4) (5) Brian Kernighan, Dennis Ritchie. _The C programming language_. Prentice Hall, Inc., Second edition, 1988. It is also commonly known as K&R and is based on the ANSI C and ISO C90 standards. (6) Bjarne Stroustrup. _The C++ programming language_. Addison-Wesley Professional; 4 edition, 2013. (7) Note that Python is good for fast programming, not fast programs. (8) For example see Jenness (2017) (https://arxiv.org/abs/1712.00461) which describes how LSST is managing the transition. (9) (10) Low-level languages are those that directly operate the hardware like assembly languages. So C is actually a high-level language, but it can be considered one of the lowest-level languages among all high-level languages. (11)  File: gnuastro.info, Node: Program design philosophy, Next: Coding conventions, Prev: Why C, Up: Developing 11.2 Program design philosophy ============================== The core processing functions of each program (and all libraries) are written mostly with the basic ISO C90 standard. We do make lots of use of the GNU additions to the C language in the GNU C library(1), but these functions are mainly used in the user interface functions (reading your inputs and preparing them prior to or after the analysis). The actual algorithms, which most scientists would be more interested in, are much more closer to ISO C90. For this reason, program source files that deal with user interface issues and those doing the actual processing are clearly separated, see *note Program source::. If anything particular to the GNU C library is used in the processing functions, it is explained in the comments in between the code. All the Gnuastro programs provide very low level and modular operations (modeled on GNU Coreutils). Almost all the basic command-line programs like ‘ls’, ‘cp’ or ‘rm’ on GNU/Linux operating systems are part of GNU Coreutils. This enables you to use shell scripting languages (for example GNU Bash) to operate on a large number of files or do very complex things through the creative combinations of these tools that the authors had never dreamed of. We have put a few simple examples in *note Tutorials::. For example all the analysis output can be saved as ASCII tables which can be fed into your favorite plotting program to inspect visually. Python’s Matplotlib is very useful for fast plotting of the tables to immediately check your results. If you want to include the plots in a document, you can use the PGFplots package within LaTeX, no attempt is made to include such operations in Gnuastro. In short, Bash can act as a glue to connect the inputs and outputs of all these various Gnuastro programs (and other programs) in any fashion. Of course, Gnuastro’s programs are just front-ends to the main workhorse (*note Gnuastro library::), allowing a user to create their own programs (for example with *note BuildProgram::). So once the functions within programs become mature enough, they will be moved within the libraries for even more general applications. The advantage of this architecture is that the programs become small and transparent: the starting and finishing point of every program is clearly demarcated. For nearly all operations on a modern computer (fast file input-output) with a modest level of complexity, the read/write speed is insignificant compared to the actual processing a program does. Therefore the complexity which arises from sharing memory in a large application is simply not worth the speed gain. Gnuastro’s design is heavily influenced from Eric Raymond’s “The Art of Unix Programmingâ€(2) which beautifully describes the design philosophy and practice which lead to the success of Unix-based operating systems(3). ---------- Footnotes ---------- (1) Gnuastro uses many GNU additions to the C library. However, thanks to the GNU Portability library (Gnulib) which is included in the Gnuastro tarball, users of non-GNU/Linux operating systems can also benefit from all these features when using Gnuastro. (2) Eric S. Raymond, 2004, _The Art of Unix Programming_, Addison-Wesley Professional Computing Series. (3) KISS principle: Keep It Simple, Stupid!  File: gnuastro.info, Node: Coding conventions, Next: Program source, Prev: Program design philosophy, Up: Developing 11.3 Coding conventions ======================= In Gnuastro, we try our best to follow the GNU coding standards. Added to those, Gnuastro defines the following conventions. It is very important for readability that the whole package follows the same convention. • The code must be easy to read by eye. So when the order of several lines within a function does not matter (for example when defining variables at the start of a function). You should put the lines in the order of increasing length and group the variables with similar types such that this half-pyramid of declarations becomes most visible. If the reader is interested, a simple search will show them the variable they are interested in. However, this visual aid greatly helps in general inspections of the code and help the reader get a grip of the function’s processing. • A function that cannot be fully displayed (vertically) in your monitor is probably too long and may be more useful if it is broken up into multiple functions. 40 lines is usually a good reference. When the start and end of a function are clearly visible in one glance, the function is much more easier to understand. This is most important for low-level functions (which usually define a lot of variables). Low-level functions do most of the processing, they will also be the most interesting part of a program for an inquiring astronomer. This convention is less important for higher level functions that don’t define too many variables and whose only purpose is to run the lower-level functions in a specific order and with checks. In general you can be very liberal in breaking up the functions into smaller parts, the GNU Compiler Collection (GCC) will automatically compile the functions as inline functions when the optimizations are turned on. So you don’t have to worry about decreasing the speed. By default Gnuastro will compile with the ‘-O3’ optimization flag. • All Gnuastro hand-written text files (C source code, Texinfo documentation source, and version control commit messages) should not exceed *75* characters per line. Monitors today are certainly much wider, but with this limit, reading the functions becomes much more easier. Also for the developers, it allows multiple files (or multiple views of one file) to be displayed beside each other on wide monitors. Emacs’s buffers are excellent for this capability, setting a buffer width of 80 with ‘’ will allow you to view and work on several files or different parts of one file using the wide monitors common today. Emacs buffers can also be used as a shell prompt and compile the program (with ), and 80 characters is the default width in most terminal emulators. If you use Emacs, Gnuastro sets the 75 character ‘fill-column’ variable automatically for you, see cartouche below. For long comments you can use press in Emacs to separate them into separate lines automatically. For long literal strings, you can use the fact that in C, two strings immediately after each other are concatenated, for example ‘"The first part, " "and the second part."’. Note the space character in the end of the first part. Since they are now separated, you can easily break a long literal string into several lines and adhere to the maximum 75 character line length policy. • The headers required by each source file (ending with ‘.c’) should be defined inside of it. All the headers a complete program needs should _not_ be stacked in another header to include in all source files (for example ‘main.h’). Although most ‘professional’ programmers choose this single header method, Gnuastro is primarily written for professional/inquisitive astronomers (who are generally amateur programmers). The list of header files included provides valuable general information and helps the reader. ‘main.h’ may only include the header file(s) that define types that the main program structure needs, see ‘main.h’ in *note Program source::. Those particular header files that are included in ‘main.h’ can of course be ignored (not included) in separate source files. • The headers should be classified (by an empty line) into separate groups: 1. ‘#include ’: This must be the first code line (not commented or blank) in each source file _within Gnuastro_. It sets macros that the GNU Portability Library (Gnulib) will use for a unified environment (GNU C Library), even when the user is building on a system that doesn’t use the GNU C library. 2. The C library header files, for example ‘stdio.h’, ‘stdlib.h’, or ‘math.h’. 3. Installed library header files, including Gnuastro’s installed headers (for example ‘cfitsio.h’ or ‘gsl/gsl_rng.h’, or ‘gnuastro/fits.h’). 4. Gnuastro’s internal headers (that are not installed), for example ‘gnuastro-internal/options.h’. 5. For programs, the ‘main.h’ file (which is needed by the next group of headers). 6. That particular program’s header files, for example ‘mkprof.h’, or ‘noisechisel.h’. As much as order does not matter when you include the header of each group, sort them by length, as described above. • All function names, variables, etc should be in lower case. Macros and constant global ‘enum’s should be in upper case. • For the naming of exported header files, functions, variables, macros, and library functions, we adopt similar conventions to those used by the GNU Scientific Library (GSL)(1). In particular, in order to avoid clashes with the names of functions and variables coming from other libraries the name-space ‘‘gal_’’ is prefixed to them. GAL stands for _G_NU _A_stronomy _L_ibrary. • All installed header files should be in the ‘lib/gnuastro’ directory (under the top Gnuastro source directory). After installation, they will be put in the ‘$prefix/include/gnuastro’ directory (see *note Installation directory:: for ‘$prefix’). Therefore with this convention Gnuastro’s headers can be included in internal (to Gnuastro) and external (a library user) source files with the same line # include Note that the GSL convention for header file names is ‘gsl_specialname.h’, so your include directive for a GSL header must be something like ‘#include ’. Gnuastro doesn’t follow this GSL guideline because of the repeated ‘gsl’ in the include directive. It can be confusing and cause bugs for beginners. All Gnuastro (and GSL) headers must be located within a unique directory and will not be mixed with other headers. Therefore the ‘‘gsl_’’ prefix to the header file names is redundant(2). • All installed functions and variables should also include the base-name of the file in which they are defined as prefix, using underscores to separate words(3). The same applies to exported macros, but in upper case. For example in Gnuastro’s top source directory, the prototype of function ‘gal_box_border_from_center’ is in ‘lib/gnuastro/box.h’, and the macro ‘GAL_POLYGON_MAX_CORNERS’ is defined in ‘lib/gnuastro/polygon.h’. This is necessary to give any user (who is not familiar with the library structure) the ability to follow the code. This convention does make the function names longer (a little harder to write), but the extra documentation it provides plays an important role in Gnuastro and is worth the cost. • There should be no trailing white space in a line. To do this automatically every time you save a file in Emacs, add the following line to your ‘~/.emacs’ file. (add-hook 'before-save-hook 'delete-trailing-whitespace) • There should be no tabs in the indentation(4). • Individual, contextually similar, functions in a source file are separated by 5 blank lines to be easily seen to be related in a group when parsing the source code by eye. In Emacs you can use . • One group of contextually similar functions in a source file is separated from another with 20 blank lines. In Emacs you can use . Each group of functions has short descriptive title of the functions in that group. This title is surrounded by asterisks (<*>) to make it clearly distinguishable. Such contextual grouping and clear title are very important for easily understanding the code. • Always read the comments before the patch of code under it. Similarly, try to add as many comments as you can regarding every patch of code. Effectively, we want someone to get a good feeling of the steps, without having to read the C code and only by reading the comments. This follows similar principles as Literate programming (https://en.wikipedia.org/wiki/Literate_programming). The last two conventions are not common and might benefit from a short discussion here. With a good experience in advanced text editor operations, the last two are redundant for a professional developer. However, recall that Gnuastro aspires to be friendly to un-familiar, and un-experienced (in programming) eyes. In other words, as discussed in *note Science and its tools::, we want the code to appear welcoming to someone who is completely new to coding (and text editors) and only has a scientific curiosity. Newcomers to coding and development, who are curious enough to venture into the code, will probably not be using (or have any knowledge of) advanced text editors. They will see the raw code in the webpage or on a simple text editor (like Gedit) as plain text. Trying to learn and understand a file with dense functions that are all spaced with one or two blank lines can be very taunting for a newcomer. But when they scroll through the file and see clear titles and meaningful spaces for similar functions, we are helping them find and focus on the part they are most interested in sooner and easier. *GNU Emacs, the recommended text editor:* GNU Emacs is an extensible and easily customizable text editor which many programmers rely on for developing due to its countless features. Among them, it allows specification of certain settings that are applied to a single file or to all files in a directory and its sub-directories. In order to harmonize code coming from different contributors, Gnuastro comes with a ‘.dir-locals.el’ file which automatically configures Emacs to satisfy most of the coding conventions above when you are using it within Gnuastro’s directories. Thus, Emacs users can readily start hacking into Gnuastro. If you are new to developing, we strongly recommend this editor. Emacs was the first project released by GNU and is still one of its flagship projects. Some resources can be found at: Official manual At . This is a great and very complete manual which is being improved for over 30 years and is the best starting point to learn it. It just requires a little patience and practice, but rest assured that you will be rewarded. If you install Emacs, you also have access to this manual on the command-line with the following command (see *note Info::). $ info emacs A guided tour of emacs At . A short visual tour of Emacs, officially maintained by the Emacs developers. Unofficial mini-manual At . A shorter manual which contains nice animated images of using Emacs. ---------- Footnotes ---------- (1) (2) For GSL, this prefix has an internal technical application: GSL’s architecture mixes installed and not-installed headers in the same directory. This prefix is used to identify their installation status. Therefore this filename prefix in GSL a technical internal issue (for developers, not users). (3) The convention to use underscores to separate words, called “snake case†(or “snake_caseâ€). This is also recommended by the GNU coding standards. (4) If you use Emacs, Gnuastro’s ‘.dir-locals.el’ file will automatically never use tabs for indentation. To make this a default in all your Emacs sessions, you can add the following line to your ‘~/.emacs’ file: ‘(setq-default indent-tabs-mode nil)’  File: gnuastro.info, Node: Program source, Next: Documentation, Prev: Coding conventions, Up: Developing 11.4 Program source =================== Besides the fact that all the programs share some functions that were explained in *note Library::, everything else about each program is completely independent. Recall that Gnuastro is written for an active astronomer/scientist (not a passive one who just uses a software). It must thus be easily navigable. Hence there are fixed source files (that contain fixed operations) that must be present in all programs, these are discussed fully in *note Mandatory source code files::. To easily understand the explanations in this section you can use *note The TEMPLATE program:: which contains the bare minimum code for one working program. This template can also be used to easily add new utilities: just copy and paste the directory and change ‘TEMPLATE’ with your program’s name. * Menu: * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program.  File: gnuastro.info, Node: Mandatory source code files, Next: The TEMPLATE program, Prev: Program source, Up: Program source 11.4.1 Mandatory source code files ---------------------------------- Some programs might need lots of source files and if there is no fixed convention, navigating them can become very hard for a new inquirer into the code. The following source files exist in every program’s source directory (which is located in ‘bin/progname’). For small programs, these files are enough. Larger programs will need more files and developers are encouraged to define any number of new files. It is just important that the following list of files exist and do what is described here. When creating other source files, please choose filenames that are a complete single word: don’t abbreviate (abbreviations are cryptic). For a minimal program containing all these files, see *note The TEMPLATE program::. ‘main.c’ Each executable has a ‘main’ function, which is located in ‘main.c’. Therefore this file is the starting point when reading any program’s source code. No actual processing functions must be defined in this file, the function(s) in this file are only meant to connect the most high level steps of each program. Generally, ‘main’ will first call the top user interface function to read user input and make all the preparations. Then it will pass control to the top processing function for that program. The functions to do both these jobs must be defined in other source files. ‘main.h’ All the major parameters which will be used in the program must be stored in a structure which is defined in ‘main.h’. The name of this structure is usually ‘prognameparams’, for example ‘cropparams’ or ‘noisechiselparams’. So ‘#include "main.h"’ will be a staple in all the source codes of the program. It is also regularly the first (and only) argument most of the program’s functions which greatly helps in readability. Keeping all the major parameters of a program in this structure has the major benefit that most functions will only need one argument: a pointer to this structure. This will significantly facilitate the job of the programmer, the inquirer and the computer. All the programs in Gnuastro are designed to be low-level, small and independent parts, so this structure should not get too large. The main root structure of all programs contains at least one instance of the ‘gal_options_common_params’ structure. This structure will keep the values to all common options in Gnuastro’s programs (see *note Common options::). This top root structure is conveniently called ‘p’ (short for parameters) by all the functions in the programs and the common options parameters within it are called ‘cp’. With this convention any reader can immediately understand where to look for the definition of one parameter. For example you know that ‘p->cp->output’ is in the common parameters while ‘p->threshold’ is in the program’s parameters. With this basic root structure, source code of functions can potentially become full of structure de-reference operators (‘->’) which can make the code very un-readable. In order to avoid this, whenever a structure element is used more than a couple of times in a function, a variable of the same type and with the same name (so it can be searched) as the desired structure element should be defined with the value of the root structure inside of it in definition time. Here is an example. char *hdu=p->cp.hdu; float threshold=p->threshold; ‘args.h’ The options particular to each program are defined in this file. Each option is defined by a block of parameters in ‘program_options’. These blocks are all you should modify in this file, leave the bottom group of definitions untouched. These are fed directly into the GNU C library’s Argp facilities and it is recommended to have a look at that for better understand what is going on, although this is not required here. Each element of the block defining an option is described under ‘argp_option’ in ‘bootstrapped/lib/argp.h’ (from Gnuastro’s top source file). Note that the last few elements of this structure are Gnuastro additions (not documented in the standard Argp manual). The values to these last elements are defined in ‘lib/gnuastro/type.h’ and ‘lib/gnuastro-internal/options.h’ (from Gnuastro’s top source directory). ‘ui.h’ Besides declaring the exported functions of ‘ui.c’, this header also keeps the “keyâ€s to every program-specific option. The first class of keys for the options that have a short-option version (single letter, see *note Options::). The character that is defined here is the option’s short option name. The list of available alphabet characters can be seen in the comments. Recall that some common options also take some characters, for those, see ‘lib/gnuastro-internal/options.h’. The second group of options are those that don’t have a short option alternative. Only the first in this group needs a value (‘1000’), the rest will be given a value by C’s ‘enum’ definition, so the actual value is irrelevant and must never be used, always use the name. ‘ui.c’ Everything related to reading the user input arguments and options, checking the configuration files and checking the consistency of the input parameters before the actual processing is run should be done in this file. Since most functions are the same, with only the internal checks and structure parameters differing. We recommend going through the ‘ui.c’ of *note The TEMPLATE program::, or several other programs for a better understanding. The most high-level function in ‘ui.c’ is named ‘ui_read_check_inputs_setup’. It accepts the raw command-line inputs and a pointer to the root structure for that program (see the explanation for ‘main.h’). This is the function that ‘main’ calls. The basic idea of the functions in this file is that the processing functions should need a minimum number of such checks. With this convention an inquirer who only wants to understand only one part (mostly the processing part and not user input details and sanity checks) of the code can easily do so in the later files. It also makes all the errors related to input appear before the processing begins which is more convenient for the user. ‘progname.c, progname.h’ The high-level processing functions in each program are in a file named ‘progname.c’, for example ‘crop.c’ or ‘noisechisel.c’. The function within these files which ‘main’ calls is also named after the program, for example void crop(struct cropparams *p) or void noisechisel(struct noisechiselparams *p) In this manner, if an inquirer is interested the processing steps, they can immediately come and check this file for the first processing step without having to go through ‘main.c’ and ‘ui.c’ first. In most situations, any failure in any step of the programs will result in an informative error message and an immediate abort in the program. So there is usually no need for return values. Under more complicated situations where a return value might be necessary, ‘void’ will be replaced with an ‘int’ in the examples above. This value must be directly returned by ‘main’, so it has to be an ‘int’. ‘authors-cite.h’ This header file keeps the global variable for the program authors and its BibTeX record for citation. They are used in the outputs of the common options ‘--version’ and ‘--cite’, see *note Operating mode options::.  File: gnuastro.info, Node: The TEMPLATE program, Prev: Mandatory source code files, Up: Program source 11.4.2 The TEMPLATE program --------------------------- The extra creativity offered by libraries comes at a cost: you have to actually write your ‘main’ function and get your hands dirty in managing user inputs: are all the necessary parameters given a value? is the input in the correct format? do the options and the inputs correspond? and many other similar checks. So when an operation has well-defined inputs and outputs and is commonly needed, it is much more worthwhile to simply do use all the great features that Gnuastro has already defined for such operations. To make it easier to learn/apply the internal program infra-structure discussed in *note Mandatory source code files::, Gnuastro ships with a template program when using the *note Version controlled source::. It is not available in the Gnuastro tarball so it doesn’t confuse people using the tarball. The ‘bin/TEMPLATE’ directory in Gnuastro’s clone contains the bare-minimum files necessary to define a new program and all the necessary files/functions are pre-defined there. You can take the following steps if you want to add a new program to Gnuastro: 1. Select a name for your new program (for example ‘myprog’). 2. Copy the ‘TEMPLATE’ directory to a directory with your program’s name: $ cp -R bin/TEMPLATE bin/myprog 3. Open ‘configure.ac’ in the top Gnuastro source. This file manages the operations that are done when a user runs ‘./configure’. Going down the file, you will notice repetitive parts for each program. Copy one of those and correct the names of the copied program to your new program name. We follow alphabetic ordering here, so please place it correctly. There are multiple places where this has to be done, so be patient and go down to the bottom of the file. Ultimately add ‘bin/myprog/Makefile’ to ‘AC_CONFIG_FILES’, only here the ordering depends on the length of the name. 4. Open ‘Makefile.am’ in the top Gnuastro source. Similar to the previous step, add your new program similar to all the other programs. 5. Change ‘TEMPLATE’ to ‘myprog’ in the file names and contents of the files in the ‘bin/myprog/’ directory. 6. Run the following command to re-build the configuration and build system. $ autoreconf -f Your new program will be built the next time you run ‘./configure’ and ‘make’. You can now start adding your special checks/processing.  File: gnuastro.info, Node: Documentation, Next: Building and debugging, Prev: Program source, Up: Developing 11.5 Documentation ================== Documentation (this book) is an integral part of Gnuastro (see *note Science and its tools::). Documentation is not considered a separate project and must be written by its developers. Users can make edits/corrections, but the initial writing must be by the developer. So, no change is considered valid for implementation unless the respective parts of the book have also been updated. The following procedure can be a good suggestion to take when you have a new idea and are about to start implementing it. The steps below are not a requirement, the important thing is that when you send the program to be included in Gnuastro, the book and the code have to both be fully up-to-date and compatible and the purpose should be very clearly explained. You can follow any path you choose to do this, the following path was what we have found to be most successful until now. 1. Edit the book and fully explain your desired change, such that your idea is completely embedded in the general context of the book with no sense of discontinuity for a first time reader. This will allow you to plan the idea much more accurately and in the general context of Gnuastro or a particular program. Later on, when you are coding, this general context will significantly help you as a road-map. A very important part of this process is the program introduction, which explains the purposes of the program. Before actually starting to code, explain your idea’s purpose thoroughly in the start of the program section you wish to add or edit. While actually writing its purpose for a new reader, you will probably get some very valuable ideas that you hadn’t thought of before. This has occurred several times during the creation of Gnuastro. If an introduction already exists, embed or blend your idea’s purpose with the existing purposes. We emphasize that doing this is equally useful for you (as the programmer) as it is useful for the user (reader). Recall that the purpose of a program is very important, see *note Program design philosophy::. As you have already noticed for every program, it is very important that the basics of the science and technique be explained in separate subsections prior to the ‘Invoking Programname’ subsection. If you are writing a new program or your addition to an existing program involves a new concept, also include such subsections and explain the concepts so a person completely unfamiliar with the concepts can get a general initial understanding. You don’t have to go deep into the details, just enough to get an interested person (with absolutely no background) started. If you feel you can’t do that, then you have probably not understood the concept yourself! If you feel you don’t have the time, then think about yourself as the reader in one year: you will forget almost all the details, so now that you have done all the theoretical preparations, add a few more hours and document it, so next time you don’t have to prepare as much. Have in mind that your only limitation in length is the fatigue of the reader after reading a long text, nothing else. So as long as you keep it relevant/interesting for the reader, there is no page number limit/cost! It might also help if you start discussing the usage of your idea in the ‘Invoking ProgramName’ subsection (explaining the options and arguments you have in mind) at this stage too. Actually starting to write it here will really help you later when you are coding. 2. After you have finished adding your initial intended plan to the book, then start coding your change or new program within the Gnuastro source files. While you are coding, you will notice that somethings should be different from what you wrote in the book (your initial plan). So correct them as you are actually coding, but don’t worry too much about missing a few things (see the next step). 3. After your work has been fully implemented, read the section documentation from the start and see if you didn’t miss any change in the coding and to see if the context is fairly continuous for a first time reader (who hasn’t seen the book or had known Gnuastro before you made your change). gnuastro-0.5/doc/gnuastro.info-30000644000175000017500000110347313217220436013576 00000000000000This is gnuastro.info, produced by makeinfo version 6.5 from gnuastro.texi. This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro’s library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: NoiseChisel, Next: MakeCatalog, Prev: Statistics, Up: Data analysis 7.2 NoiseChisel =============== Once instrumental signatures are removed from the raw data in the initial reduction process (see *note Data manipulation::). We are ready to derive scientific results out of them. But we can’t do anything special with a raw dataset, for example an image is just an array of values. Every pixel just has one value and its position within the image. Therefore, the first step of your high-level analysis will be to classify/label the dataset elements/pixels into two classes: signal and noise. This process is formally known as _detection_. Afterwards, you want to separate the detections into multiple components (for example when two detected regions aren’t touching, they should be treated independently as two distant galaxies for example). This higher level classification of the detections is known as _segmentation_. NoiseChisel is Gnuastro’s program for detection and segmentation. NoiseChisel works based on a new noise-based approach to signal detection and was introduced to the astronomical community in Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664). NoiseChisel’s primary output is an array (image) with the same size as the input but containing labels: those pixels with a label of 0 are noise/sky while those pixels with labels larger than 0 are detections (separate segments will be given positive integers, starting from 1). For more on NoiseChisel’s particular output format and its benefits (especially in conjunction with *note MakeCatalog::), please see Akhlaghi [2016] (https://arxiv.org/abs/1611.06387). The published paper cannot under go any updates, but the NoiseChisel software has evolved, you can see the major changes in *note NoiseChisel changes after publication::. Data is inherently mixed with noise: only mock/simulated datasets are free of noise. So this process of separating signal from noise is not trivial. In particular, most scientifically interesting astronomical targets are faint, can have a large variety of morphologies along with a large distribution in brightness and size which are all drowned in a ocean of noise. So detection is a uniquely vital aspect of any scientific work and even more so for astronomical research. This is such a fundamental step that designing of NoiseChisel was the primary motivation behind creating Gnuastro: the first generation of Gnuastro’s programs were all first part of what later became NoiseChisel, afterwards they spinned-off into separate programs. The name of NoiseChisel is derived from the first thing it does after thresholding the dataset: to erode it. In mathematical morphology, erosion on pixels can be pictured as carving off boundary pixels. Hence, what NoiseChisel does is similar to what a wood chisel or stone chisel do. It is just not a hardware, but a software. In fact looking at it as a chisel and your dataset as a solid cube of rock will greatly help in best using it: with NoiseChisel you literally carve the galaxies/stars/comets out of the noise. Try running it with the ‘--checkdetection’ option to see each step of the carving process on your input dataset. You can then change a specific option to carve out your signal out of the noise more successfully. * Menu: * NoiseChisel changes after publication:: Changes to the software after publication. * Invoking astnoisechisel:: Options and arguments for NoiseChisel.  File: gnuastro.info, Node: NoiseChisel changes after publication, Next: Invoking astnoisechisel, Prev: NoiseChisel, Up: NoiseChisel 7.2.1 NoiseChisel changes after publication ------------------------------------------- Before using NoiseChisel it is strongly recommended to read Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664) to gain a good understanding of what it does and how each parameter influences the output. Thanks to that paper, there is no need to go into the details of the major processing steps. Hence we can just dive into the details of running NoiseChisel in *note Invoking astnoisechisel::. However, the paper cannot undergo any further updates, but NoiseChisel will evolve: better algorithms or steps will be found, thus options will be added or removed. So this book is the final and definitive guide. For a more detailed list of changes in each release, please follow the ‘NEWS’ file. The ‘NEWS’ file is in the released Gnuastro tarball (see *note Release tarball::). You can also view the most recent ‘NEWS’ file online (http://git.savannah.gnu.org/cgit/gnuastro.git/plain/NEWS)(1). To make the transition form the paper to this book easier (and encourage reading the paper), below you can see the major changes since the paper was published. First, the options that have been removed are discussed, followed by those that have been added. Removed options: • ‘--dilate’: In the paper, true detections were dilated for a final dig into the noise. However, simple 8-connected dilation can produce boxy results which are not realistic and could miss diffuse flux. The final dig into the noise is now done by “growâ€ing the true detections, similar to how true clumps were grown, see the description of ‘--detgrowquant’ below and in *note Detection options:: for more on the new alternative. Added options: • ‘--widekernel’: NoiseChisel uses the difference between the mode and median to identify if a tile should be used for estimating the quantile thresholds (see *note Quantifying signal in a tile::). Until now, NoiseChisel would convolve an image once and estimate the proper tiles for quantile estimations on the convolved image. The same convolved image would later be used for quantile estimation. A larger kernel does increase the skewness (and thus difference between the mode and median), however, it disfigures the shapes/morphology of the objects. This new ‘--widekernel’ option (and a corresponding ‘--wkhdu’ option to specify its HDU) option are added to solve such cases. When its given, the input will be convolved with both the sharp (given through the ‘--kernel’ option) and wide kernels. The mode and median are calculated on the dataset that is convolved with the wider kernel, then the quantiles are estimated on the image convolved with the sharper kernel. • ‘--noerodequant’: to specify a quantile threshold where erosion will not apply. This is useful to detect sharper point-like sources that will be missed due to too much erosion. To completely ignore this features give this option a value of 1 (only the largest valued pixel in the input will not be eroded). • ‘--qthreshtilequant’: to manually remove the measured qthresh from some tiles. This feature helps in detecting large and extended diffuse (almost flat) signal when necessary, see *note Detection options::. • ‘--detgrowquant’: is used to grow the final true detections until a given quantile in the same way that clumps are grown during segmentation (compare columns 2 and 3 in Figure 10 of the paper). It replaces the old ‘--dilate’ option in the paper and older versions of Gnuastro. Dilation is a blind growth method which causes objects to be boxy or diamond shaped when too many layers are added. However, with the growth method that is defined now, we can follow the signal into the noise with any shape. The appropriate quantile depends on your dataset’s correlated noise properties and how cleanly it was Sky subtracted. The new ‘--detgrowmaxholesize’ can also be used to specify the maximum hole size to fill as part of this growth, see the description in *note Detection options:: for more details. This new growth process can be much more successful in detecting diffuse flux around true detections compared to dilation and give more realistic results, but it can also increase the NoiseChisel run time (depending on the given value and input size). • ‘--cleangrowndet’: A process to further clean/remove the possibility of false detections, see the descriptions under this option in *note Detection options::. ---------- Footnotes ---------- (1) The online version of the ‘NEWS’ file here may contain features that have been implemented, but not yet officially released as a tarball (see *note Downloading the source::). Therefore, please be sure to look at the dates and versions above each group of changed features and make sure it corresponds to your installed version. It is hence recommended to always stay up to date, see *note Announcements::).  File: gnuastro.info, Node: Invoking astnoisechisel, Prev: NoiseChisel changes after publication, Up: NoiseChisel 7.2.2 Invoking NoiseChisel -------------------------- NoiseChisel will detect and segment signal in noise producing a multi-extension labeled image, ready for input into *note MakeCatalog:: to generate a catalog or other processing. The executable name is ‘astnoisechisel’ with the following general template $ astnoisechisel [OPTION ...] InputImage.fits One line examples: ## Detect signal in input.fits: $ astnoisechisel input.fits ## Detect signal assuming input has 4 channels along first dimension ## and 1 along the second. Also set the regular tile size to 100 along ## both dimensions: $ astnoisechisel --numchannels=4,1 --tilesize=100,100 input.fits If NoiseChisel is to do processing (for example you don’t want to get help, or see the values to each input parameter), an input image should be provided with the recognized extensions (see *note Arguments::). NoiseChisel shares a large set of common operations with other Gnuastro programs, mainly regarding input/output, general processing steps, and general operating modes. To help in a unified experience between all of Gnuastro’s programs, these operations have the same command-line options, see *note Common options:: for a full list. Since the common options are thoroughly discussed there, they are no longer reviewed here. You can see all the options with a short description on the command-line with the ‘--help’ option, see *note Getting help::. NoiseChisel’s input image may contain blank elements (see *note Blank pixels::). Blank elements will be ignored in all steps of NoiseChisel. Hence if your dataset has bad pixels which should be masked with a mask image, please use Gnuastro’s *note Arithmetic:: program (in particular its ‘where’ operator) to convert those pixels to blank pixels before running NoiseChisel. Gnuastro’s Arithmetic program has bitwise operators helping you select specific kinds of bad-pixels when necessary. A convolution kernel can also be optionally given. If a value (file name) is given to ‘--kernel’ on the command-line or in a configuration file (see *note Configuration files::), then that file will be used to convolve the image prior to thresholding. Otherwise a default kernel will be used. The default kernel is a 2D Gaussian with a FWHM of 2 pixels truncated at 5 times the FWHM. This choice of the default kernel is discussed in Section 3.1.1 of Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664). See *note Convolution kernel:: for kernel related options. NoiseChisel defines two tessellations over the input (see *note Tessellation::). This enables it to deal with possible gradients in the input dataset and also significantly improve speed by processing each tile on different threads. The tessellation related options are discussed in *note Processing options::. In particular, NoiseChisel uses two tessellations (with everything between them identical except the tile sizes): a fine-grained one with smaller tiles (mainly used in detection) and a more larger tiled one which is used for multi-threaded processing. The common Tessellation options described in *note Processing options:: define all parameters of both tessellations, only the large tile size for the latter tessellation is set through the ‘--largetilesize’ option. To inspect the tessellations on your input dataset, run NoiseChisel with ‘--checktiles’. *Usage TIP:* Frequently use the options starting with ‘--check’. Depending on what you want to detect in the data, you can often play with the parameters/options for a better result than the default parameters. You can start with ‘--checkdetection’ and ‘--checksegmentation’ for the main steps. For their full list please run: $ astnoisechisel --help | grep check In the sections below, NoiseChisel’s options are classified into three general classes to help in easy navigation. *note General NoiseChisel options:: mainly discusses the options relating to input and those that are shared in both detection and segmentation. Options to configure the detection are described in *note Detection options:: and *note Segmentation options:: we discuss how you can fine-tune the segmentation of the detections. Finally in *note NoiseChisel output:: the format of NoiseChisel’s output is discussed. The order of options here follow the same logical order that the respective action takes place within NoiseChisel (note that the output of ‘--help’ is sorted alphabetically). * Menu: * General NoiseChisel options:: General NoiseChisel preprocessing. * Detection options:: Configure detection in NoiseChisel. * Segmentation options:: Configure segmentation in NoiseChisel. * NoiseChisel output:: NoiseChisel’s output format.  File: gnuastro.info, Node: General NoiseChisel options, Next: Detection options, Prev: Invoking astnoisechisel, Up: Invoking astnoisechisel 7.2.2.1 General NoiseChisel options ................................... The options discussed in this section are mainly regarding the input(s), output, and some general processing options that are shared between both detection and segmentation. Recall that you can always see the full list of Gnuastro’s options with the ‘--help’ option. ‘-k STR’ ‘--kernel=STR’ File name of kernel to smooth the image before applying the threshold, see *note Convolution kernel::. The first step of NoiseChisel is to convolve/smooth the image and use the convolved image in multiple steps during the processing. It will be used to define (and later apply) the quantile threshold (see ‘--qthresh’). The convolved image is also used to define the clumps (see Section 3.2.1 and Figure 8 of Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664)). The ‘--kernel’ option is not mandatory. If no kernel is provided, a 2D Gaussian profile with a FWHM of 2 pixels truncated at 5 times the FWHM is used. This choice of the default kernel is discussed in Section 3.1.1 of Akhlaghi and Ichikawa [2015]. ‘--khdu=STR’ HDU containing the kernel in the file given to the ‘--kernel’ option. ‘--convolved=STR’ Use this file as the convolved image and don’t do convolution and ignore ‘--kernel’. NoiseChisel will just check the size of the given dataset is the same as the input’s size. If a wrong image (with the same size) is given to this option, the results (errors, bugs, and etc) are un-predictable. So please use this option with care and in a highly controlled environment. On such scenario is discussed below. In almost all situations, as the input gets larger, the single most CPU and time consuming step in NoiseChisel is convolution (the first step in its processing). The process of testing NoiseChisel for the best parameters in a given analysis will involve running NoiseChisel multiple times: to see the effect of each new option value. Therefore, once the kernel is finalized, re-convolving the input will greatly hinder fast testing of higher-level parameters. With this option, you can convolve the input image with your chosen kernel once before running NoiseChisel, then feed it to NoiseChisel on each test run and thus save valuable time for better/more tests. To build your desired convolution kernel, you can use *note MakeProfiles::. To convolve the image with a given kernel you can use *note Convolve::. Spatial domain convolution is mandatory. In the frequency domain, blank pixels (if present) will cover the whole image and gradients will appear on the edges, see *note Spatial vs. Frequency domain::. Below you can see an example of such a scenario: you want to see how variation of the growth level (through the ‘--detgrowquant’ option) will affect the final result. Recall that you can ignore all the extra spaces, new lines, and ‘‘\’’ if you are typing in the terminal (in a shell script, remove the ‘$’ signs at the start of the lines). ## Make the kernel to convolve with. $ astmkprof --oversample=1 --kernel=gaussian,2,5 ## Convolve the input with the given kernel. $ astconvolve input.fits --kernel=kernel.fits \ --domain=spatial --output=convolved.fits ## Run NoiseChisel with seven growth quantile values. $ for g in 60 65 70 75 80 85 90; do \ astnoisechisel input.fits --convolved=convolved.fits \ --detgrowquant=0.$g --output=$g.fits; \ done ‘--convolvedhdu=STR’ The HDU/extension containing the convolved image in the file given to ‘--convolved’. ‘-w STR’ ‘--widekernel=STR’ File name of a wider kernel to use in estimating the difference of the mode and median in a tile (this difference is used to identify the significance of signal in that tile, see *note Quantifying signal in a tile::). This convolved image is only used for this purpose. Once the mode is found to be sufficiently close to the median, the input convolved with the sharper kernel (‘--kernel’) is used to identify the quantile threshold (see ‘--qthresh’). Since this convolution will significantly slow down the processing, it is optional. If no image is given, the mode and median will be found on the image that is convolved with the dataset in ‘--kernel’. ‘--wkhdu=STR’ HDU containing the kernel file given to the ‘--widekernel’ option. ‘-E’ ‘--skysubtracted’ If this option is called, it is assumed that the image has already been sky subtracted once. Knowing if the sky has already been subtracted once or not is very important in estimating the Signal to noise ratio of the detections and clumps. In short an extra $\sigma_{sky}^2$ must be added in the error (noise or denominator in the Signal to noise ratio) for every flux value that is present in the calculation. This can be interpreted as the error in measuring that sky value when it was subtracted by any other program. See Section 3.3 in Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664)) for a complete explanation. ‘-B FLT’ ‘--minskyfrac=FLT’ Minimum fraction (value between 0 and 1) of sky (undetected) areas in a tile for it to be considered in measuring the following detection and segmentation properties. • Measuring the Signal to noise ratio of false detections during the false detection removal on small tiles. • Measuring the sky value (average of undetected pixels) on small tiles. Both before the removal of false detections and after it. • Clump Signal to noise ratio in the sky regions of large files. Because of the PSF and their intrinsic amorphous properties, astronomical objects (except cosmic rays) never have a clear cutoff and commonly sink into the noise very slowly. Even below the very low thresholds used by NoiseChisel. So when a large fraction of the area of one mesh is covered by detections, it is very plausible that their faint wings are present in the undetected regions (hence causing a bias in any measurement). To get an accurate measurement of the above parameters over the tessellation, tiles that harbor too many detected regions should be excluded. The used tiles are visible in the respective ‘--check’ option of the given step. ‘--minnumfalse=INT’ The minimum number of ‘pseudo-detections’ (to identify false initial detections) or clumps (to identifying false clumps) found over the un-detected regions to identify a Signal-to-Noise ratio threshold. The Signal to noise ratio (S/N) of false pseudo-detections and clumps in each tile is found using the quantile of the S/N distribution of the psudo-detections and clumps over the undetected pixels in each mesh. If the number of S/N measurements is not large enough, the quantile will not be accurate (can have large scatter). For example if you set ‘--detquant=0.99’ (or the top 1 percent), then it is best to have at least 100 S/N measurements. ‘-L INT[,INT]’ ‘--largetilesize=INT[,INT]’ The size of each tile for the tessellation with the larger tile sizes. Except for the tile size, all the other parameters for this tessellation are taken from the common options described in *note Processing options::. The format is identical to that of the ‘--tilesize’ option that is discussed in that section. ‘--onlydetection’ If this option is called, no segmentation will be done and the output will only have four extensions (no clumps extension, see *note NoiseChisel output::). The second extension of the output is not going to be objects but raw detections (a large region will be given one label): labeling is only done based on connectivity. The last two extensions of the output will be the Sky and its Standard deviation. This option can result in faster processing when only the noise properties of the image are desired for a catalog using another image’s labels for example. A common case is when you want to measure colors or SEDs in several images. Let’s say you have images in two colors: A and B. For simplicity also assume that they are exactly on the same position in the sky with the same pixel scale. You choose to set A as a reference, so you run the NoiseChisel fully on A. Then you run NoiseChisel on B with ‘--onlydetection’ since you only need the noise properties of B (for the signal to noise column in its catalog). You can then run MakeCatalog on A normally, see *note MakeCatalog::. To run MakeCatalog on B, you simply set the object and clump labels images to those that NoiseChisel produced for A, see *note Invoking astmkcatalog::. ‘--continueaftercheck’ Continue NoiseChisel after any of the options starting with ‘--check’. NoiseChisel involves many steps and as a result, there are many checks, allowing to inspect the status of the processing. The results of each step affect the next steps of processing, so, when you are want to check the status of the processing at one step, the time spent to complete NoiseChisel is just wasted/distracting time. To encourage easier experimentation with the option values, when you use any of the NoiseChisel options that start with ‘--check’, NoiseChisel will abort once all the desired check file(s) is (are) completed. If you call the ‘--continueaftercheck’ option, you can disable this behavior and ask NoiseChisel to continue with the rest of the processing after completing the check file(s).  File: gnuastro.info, Node: Detection options, Next: Segmentation options, Prev: General NoiseChisel options, Up: Invoking astnoisechisel 7.2.2.2 Detection options ......................... Detection is the process of separating the pixels in the image into two groups: 1) Signal and 2) Noise. Through the parameters below, you can customize the detection process in NoiseChisel. Recall that you can always see the full list of Gnuastro’s options with the ‘--help’ option. ‘-r FLT’ ‘--mirrordist=FLT’ Maximum distance (as a multiple of error) to estimate the difference between the input and mirror distributions in finding the mode, see Appendix C of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664), also see *note Quantifying signal in a tile::. ‘-Q FLT’ ‘--modmedqdiff=FLT’ The maximum acceptable distance between the mode and median, see *note Quantifying signal in a tile::. The quantile threshold will be found on tiles that satisfy this mode and median difference. ‘-t FLT’ ‘--qthresh=FLT’ The quantile threshold to apply to the convolved image. The detection process begins with applying a quantile threshold to each of the tiles in the small tessellation. The quantile is only calculated for tiles that don’t have any significant signal within them, see *note Quantifying signal in a tile::. Interpolation is then used to give a value to the un-successful tiles and it is finally smoothed. The quantile value is a floating point value between 0 and 1. Assume that we have sorted the $N$ data elements of a distribution (the pixels in each mesh on the convolved image). The quantile ($q$) of this distribution is the value of the element with an index of (the nearest integer to) $q\times{N}$ in the sorted data set. After thresholding is complete, we will have a binary (two valued) image. The pixels above the threshold are known as foreground pixels (have a value of 1) while those which lie below the threshold are known as background (have a value of 0). ‘--qthreshtilequant=FLT’ Only keep tiles which have a q-thresh value above the given quantile of the all successful tiles. Hence, when given a value of ‘1’, this option will be ignored. When there is more than one channel (and ‘--workoverch’ is not called), quantile calculation and application will be done on each channel independently. This option is useful when a large and diffuse (almost flat within each tile) signal exists with very small regions of Sky. The flatness of the profile will cause it to successfully pass the tests of *note Quantifying signal in a tile::. As a result, without this option the flat and diffuse signal will be interpretted as sky. In such cases, you can see the status of the tiles with the ‘--checkqthresh’ option (first image extension is enough) and select a quantile through this option to ignore the measured values in the higher-valued tiles. This option can also be useful when there are large bright objects in the image with large flat wings which can also pass the tests and give outlier values. When there is a sky gradient over the image (mainly due to post-processing issues like bad flat fielding), this option must be set to ‘1’ so it is completely ignored and the sky gradient is accurately measured and subtracted. To get an estimate of the measured qthresh distribution, you can run the following commands. The first will create the qthresh check image with one value/pixel per tile (see *note Processing options::). Open the image in a FITS viewer and inspect it. The second command below will print the basic information about the distribution of values and the third will print the value at the 0.4 quantile. Recall that Gnuastro’s Statistics program ignores blank values (in this case: tiles with significant signal), see *note Statistics::. $ astnoisechisel image.fits --checkqthresh --oneelempertile $ aststatistics image_qthresh.fits $ aststatistics image_qthresh.fits --quantile=0.4 ‘--smoothwidth=INT’ Width of flat kernel used to smooth the interpolated quantile thresholds, see ‘--qthresh’ for more. ‘--checkqthresh’ Check the quantile threshold values on the mesh grid. A file suffixed with ‘_qthresh.fits’ will be created showing each step. With this option, NoiseChisel will abort as soon as quantile estimation has been completed, allowing you to inspect the steps leading to the final quantile threshold, this can be disabled with ‘--continueaftercheck’. By default the output will have the same pixel size as the input, but with the ‘--oneelempertile’ option, only one pixel will be used for each tile (see *note Processing options::). ‘-e INT’ ‘--erode=INT’ The number of erosions to apply to the binary thresholded image. Erosion is simply the process of flipping (from 1 to 0) any of the foreground pixels that neighbor a background pixel. In a 2D image, there are two kinds of neighbors, 4-connected and 8-connected neighbors. You can specify which type of neighbors should be used for erosion with the ‘--erodengb’ option, see below. Erosion has the effect of shrinking the foreground pixels. To put it another way, it expands the holes. This is a founding principle in NoiseChisel: it exploits the fact that with very low thresholds, the holes in the very low surface brightness regions of an image will be smaller than regions that have no signal. Therefore by expanding those holes, we are able to separate the regions harboring signal. ‘--erodengb=INT’ The type of neighborhood (structuring element) used in erosion, see ‘--erode’ for an explanation on erosion. Only two integer values are acceptable: 4 or 8. In 4-connectivity, the neighbors of a pixel are defined as the four pixels on the top, bottom, right and left of a pixel that share an edge with it. The 8-connected neighbors on the other hand include the 4-connected neighbors along with the other 4 pixels that share a corner with this pixel. See Figure 6 (a) and (b) in Akhlaghi and Ichikawa (2015) for a demonstration. ‘--noerodequant’ Pure erosion is going to carve off sharp and small objects completely out of the detected regions. This option can be used to avoid missing such sharp and small objects (which have significant pixels, but not over a large area). All pixels with a value larger than the significance level specified by this option will not be eroded during the erosion step above. However, they will undergo the erosion and dilation of the opening step below. Like the ‘--qthresh’ option, the significance level is determined using the quantile (a value between 0 and 1). Just as a reminder, in the normal distribution, $1\sigma$, $1.5\sigma$, and $2\sigma$ are approximately on the 0.84, 0.93, and 0.98 quantiles. ‘-p INT’ ‘--opening=INT’ Depth of opening to be applied to the eroded binary image. Opening is a composite operation. When opening a binary image with a depth of $n$, $n$ erosions (explained in ‘--erode’) are followed by $n$ dilations. Simply put, dilation is the inverse of erosion. When dilating an image any background pixel is flipped (from 0 to 1) to become a foreground pixel. Dilation has the effect of fattening the foreground. Note that in NoiseChisel, the erosion which is part of opening is independent of the initial erosion that is done on the thresholded image (explained in ‘--erode’). The structuring element for the opening can be specified with the ‘--openingngb’ option. Opening has the effect of removing the thin foreground connections (mostly noise) between separate foreground ‘islands’ (detections) thereby completely isolating them. Once opening is complete, we have _initial_ detections. ‘--openingngb=INT’ The structuring element used for opening, see ‘--erodengb’ for more information about a structuring element. ‘-s FLT,FLT’ ‘--sigmaclip=FLT,FLT’ The $\sigma$-clipping parameters, see *note Sigma clipping::. This option takes two values which are separated by a comma (<,>). Each value can either be written as a single number or as a fraction of two numbers (for example ‘3,1/10’). The first value to this option is the multiple of $\sigma$ that will be clipped ($\alpha$ in that section). The second value is the exit criteria. If it is less than 1, then it is interpreted as tolerance and if it is larger than one it is assumed to be the fixed number of iterations. Hence, in the latter case the value must be an integer. ‘--checkdetsky’ Check the initial approximation of the sky value and its standard deviation in a FITS file ending with ‘_detsky.fits’. With this option, NoiseChisel will abort as soon as the sky value used for defining pseudo-detections is complete. This allows you to inspect the steps leading to the final quantile threshold, this behavior can be disabled with ‘--continueaftercheck’. By default the output will have the same pixel size as the input, but with the ‘--oneelempertile’ option, only one pixel will be used for each tile (see *note Processing options::). ‘-R FLT’ ‘--dthresh=FLT’ The detection threshold: a multiple of the initial sky standard deviation added with the initial sky approximation (which you can inspect with ‘--checkdetsky’). This flux threshold is applied to the initially undetected regions on the un-convolved image. The background pixels that are completely engulfed in a 4-connected foreground region are converted to background (holes are filled) and one opening (depth of 1) is applied over both the initially detected and undetected regions. The Signal to noise ratio of the resulting ‘psudo-detections’ are used to identify true vs. false detections. See Section 3.1.5 and Figure 7 in Akhlaghi and Ichikawa (2015) for a very complete explanation. ‘-i INT’ ‘--detsnminarea=INT’ The minimum area to calculate the Signal to noise ratio on the psudo-detections of both the initially detected and undetected regions. When the area in a psudo-detection is too small, the Signal to noise ratio measurements will not be accurate and their distribution will be heavily skewed to the positive. So it is best to ignore any psudo-detection that is smaller than this area. Use ‘--detsnhistnbins’ to check if this value is reasonable or not. ‘--checkdetsn’ Save the S/N values of the pseudo-detections and dilated detections into three files ending with ‘_detsn_sky.XXX’, ‘_detsn_det.XXX’, and ‘_detsn_dilated.XXX’. The ‘.XXX’ is determined from the ‘--tableformat’ option (see *note Input output options::, for example ‘.txt’ or ‘.fits’). You can use these to inspect the S/N values and their distribution (in combination with the ‘--checkdetection’ option to see where the pseudo-detections are). You can use Gnuastro’s *note Statistics:: to make a histogram of the distribution or any other analysis you would like for better understanding of the distribution (for example through a histogram). With this option, NoiseChisel will abort as soon as the tables are created. This allows you to inspect the steps leading to the final quantile threshold, this behavior (to abort NoiseChisel) can be disabled with ‘--continueaftercheck’. ‘-c FLT’ ‘--detquant=FLT’ The quantile of the Signal to noise ratio distribution of the psudo-detections in each mesh to use for filling the large mesh grid. Note that this is only calculated for the large mesh grids that satisfy the minimum fraction of undetected pixels (value of ‘--minbfrac’) and minimum number of psudo-detections (value of ‘--minnumfalse’). ‘-d FLT’ ‘--detgrowquant=FLT’ Quantile limit to “grow†the final detections. As discussed in the previous options, after applying the initial quantile threshold, layers of pixels are carved off the objects to identify true signal. With this step you can return those low surface brightness layers that were carved off back to the detections. To disable growth, set the value of this option to ‘1’. The process is as follows: after the true detections are found, all the non-detected pixels above this quantile will be put in a list and used to “grow†the true detections (seeds of the growth). Like all quantile thresholds, this threshold is defined and applied to the convolved dataset. Afterwards, the dataset is dilated once (with minimum connectivity) to connect very thin regions on the boundary: imagine building a dam at the point rivers spill into an open sea/ocean. Finally, all holes are filled. In the geography metaphor, holes can be seen as the closed (by the dams) rivers and lakes, so this process is like turning the water in all such rivers and lakes into soil. See ‘--detgrowmaxholesize’ for configuring the hole filling. ‘--detgrowmaxholesize=INT’ The maximum hole size to fill during the final expansion of the true detections as described in ‘--detgrowquant’. This is necessary when the input contains many smaller objects and can be used to avoid marking blank sky regions as detections. For example multiple galaxies can be positioned such that they surround an empty region of sky. If all the holes are filled, the Sky region in between them will be taken as a detection which is not desired. To avoid such cases, the integer given to this option must be smaller than the hole between the objects. On the other hand, if you have a very large (and extended) galaxy, the diffuse wings of the galaxy may create very large holes. In such cases, a larger value to this option will cause the whole region to be detected as part of the large galaxy and thus detect it to extremely low surface brightness limits. ‘--cleangrowndet’ After dilation, if the signal-to-noise ratio of a detection is less than the derived pseudo-detection S/N limit, that detection will be discarded. In an ideal/clean noise, a true detection’s S/N should be larger than its constituent pseudo-detections because its area is larger and it also covers more signal. However, on a false detections (especially at lower ‘--detquant’ values), the increase in size can cause a decrease in S/N below that threshold. This will improve purity and not change completeness (a true detection will not be discarded). Because a true detection has flux in its vicinity and dilation will catch more of that flux and increase the S/N. So on a true detection, the final S/N cannot be less than pseudo-detections. However, in many real images bad processing creates artifacts that cannot be accurately removed by the Sky subtraction. In such cases, this option will decrease the completeness (will artificially discard true detections). So this feature is not default and should to be explicitly called when you know the noise is clean. ‘--checkdetection’ Every step of the detection process will be added as an extension to a file with the suffix ‘_det.fits’. Going through each would just be a repeat of the explanations above and also of those in Akhlaghi and Ichikawa (2015). The extension label should be sufficient to recognize which step you are observing. Viewing all the steps can be the best guide in choosing the best set of parameters. With this option, NoiseChisel will abort as soon as a snapshot of all the detection process is saved. This behavior can be disabled with ‘--continueaftercheck’. ‘--checksky’ Check the derivation of the final sky and its standard deviation values on the mesh grid. With this option, NoiseChisel will abort as soon as the sky value is estimated over the image (on each tile). This behavior can be disabled with ‘--continueaftercheck’. By default the output will have the same pixel size as the input, but with the ‘--oneelempertile’ option, only one pixel will be used for each tile (see *note Processing options::).  File: gnuastro.info, Node: Segmentation options, Next: NoiseChisel output, Prev: Detection options, Up: Invoking astnoisechisel 7.2.2.3 Segmentation options ............................ Segmentation is the process of (possibly) breaking up a detection into multiple segments (technically called _objects_ and _clumps_ in NoiseChisel). In deep surveys segmentation becomes particularly important because we will be detecting more diffuse flux so galaxy images are going to overlap more. It is thus very important to be able separate the pixels within a detection. In NoiseChisel, segmentation is done by first finding the ‘true’ clumps over a detection and then expanding those clumps to a certain flux limit. True clumps are found in a process very similar to the true detections explained in *note Detection options::, see Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664) for more information. If the connections between the grown clumps are weaker than a given threshold, the grown clumps are considered to be separate objects. ‘-m INT’ ‘--segsnminarea=INT’ The minimum area which a clump in the undetected regions should have in order to be considered in the clump Signal to noise ratio measurement. If this size is set to a small value, the Signal to noise ratio of false clumps will not be accurately found. It is recommended that this value be larger than the value to ‘--detsnminarea’. Because the clumps are found on the convolved (smoothed) image while the psudo-detections are found on the input image. You can use ‘--checkclumpsn’ and ‘--checksegmentation’ to see if your chosen value is reasonable or not. ‘--checkclumpsn’ Save the S/N values of the clumps into two files ending with ‘_clumpsn_sky.XXX’ and ‘_clumpsn_det.XXX’. The ‘.XXX’ is determined from the ‘--tableformat’ option (see *note Input output options::, for example ‘.txt’ or ‘.fits’). You can use these to inspect the S/N values and their distribution (in combination with the ‘--checksegmentation’ option to see where the clumps are). You can use Gnuastro’s *note Statistics:: to make a histogram of the distribution (ready for plotting in a text file, or a crude ASCII-art demonstration on the command-line). With this option, NoiseChisel will abort as soon as the two tables are created. This allows you to inspect the steps leading to the final S/N quantile threshold, this behavior can be disabled with ‘--continueaftercheck’. ‘-g FLT’ ‘--segquant=FLT’ The quantile of the noise clump Signal to noise ratio distribution. This value is used to identify true clumps over the detected regions. You can get the full distribution of clumps S/Ns over the undetected areas with the ‘--checkclumpsn’ option and see them with ‘--checksegmentation’. ‘-v’ ‘--keepmaxnearriver’ Keep a clump whose maximum flux is 8-connected to a river pixel. By default such clumps over detections are considered to be noise and are removed irrespective of their brightness (see *note Flux Brightness and magnitude::). Over large profiles, that sink into the noise very slowly, noise can cause part of the profile (which was flat without noise) to become a very large and with a very high Signal to noise ratio. In such cases, the pixel with the maximum flux in the clump will be immediately touching a river pixel. ‘-G FLT’ ‘--gthresh=FLT’ Threshold (multiple of the sky standard deviation added with the sky) to stop growing true clumps. Once true clumps are found, they are set as the basis to segment the detected region. They are grown until the threshold specified by this option. ‘-y INT’ ‘--minriverlength=INT’ The minimum length of a river between two grown clumps for it to be considered in Signal to noise ratio estimations. Similar to ‘--segsnminarea’ and ‘--detsnminarea’, if the length of the river is too short, the Signal to noise ratio can be noisy and unreliable. Any existing rivers shorter than this length will be considered as non-existent, independent of their Signal to noise ratio. Since the clumps are grown on the input image, this value should best be similar to the value of ‘--detsnminarea’. Recall that the clumps were defined on the convolved image so ‘--segsnminarea’ was larger than ‘--detsnminarea’. ‘-O FLT’ ‘--objbordersn=FLT’ The maximum Signal to noise ratio of the rivers between two grown clumps in order to consider them as separate ‘objects’. If the Signal to noise ratio of the river between two grown clumps is larger than this value, they are defined to be part of one ‘object’. Note that the physical reality of these ‘objects’ can never be established with one image, or even multiple images from one broad-band filter. Any method we devise to define ‘object’s over a detected region is ultimately subjective. Two very distant galaxies or satellites in one halo might lie in the same line of sight and be detected as clumps on one detection. On the other hand, the connection (through a spiral arm or tidal tail for example) between two parts of one galaxy might have such a low surface brightness that they are broken up into multiple detections or objects. In fact if you have noticed, exactly for this purpose, this is the only Signal to noise ratio that the user gives into NoiseChisel. The ‘true’ detections and clumps can be objectively identified from the noise characteristics of the image, so you don’t have to give any hand input Signal to noise ratio. ‘--grownclumps’ In the output (see *note NoiseChisel output::) store the grown clumps (or full detected region if only one clump was present in that detection). By default the original clumps are stored as the third extension of the output, if this option is called, it is replaced with the grown clump labels. ‘--checksegmentation’ A file with the suffix ‘_seg.fits’ will be created. This file keeps all the relevant steps in finding true clumps and segmenting the detections into multiple objects in various extensions. Having read the paper or the steps above. Examining this file can be an excellent guide in choosing the best set of parameters. Note that calling this function will significantly slow NoiseChisel. In verbose mode (without the ‘--quiet’ option, see *note Operating mode options::) the important steps (along with their extension names) will also be reported. With this option, NoiseChisel will abort as soon as the two tables are created. This behavior can be disabled with ‘--continueaftercheck’.  File: gnuastro.info, Node: NoiseChisel output, Prev: Segmentation options, Up: Invoking astnoisechisel 7.2.2.4 NoiseChisel output .......................... The default name and directory of the outputs are explained in *note Automatic output::. NoiseChisel’s default output (when none of the options starting with ‘--check’ or the ‘--output’ option are called) is one file ending with ‘_labeled.fits’. This file has the extensions listed below: 1. A copy of the input image, a copy is placed here for the following reasons: • By flipping through the extensions, a user can check how accurate the detection and segmentation process was. • All the inputs to MakeCatalog (see *note MakeCatalog::) are included in this one file which makes the running of MakeCatalog after NoiseChisel very easy. 2. The object/detection labels. Each pixel in the input image is given a label in this extension, the labels start from one. If the ‘--onlydetection’ option is given, each large connected part of the image has one label. Without that option, this extension is going to show the labels of the objects that are found after segmentation. The total number of labels is stored as the value to the ‘NOBJS’/‘NDETS’ keyword in the header of this extension. This number is also printed in verbose mode. 3. The clump labels when ‘--onlydetection’ is not called. All the pixels in the input image that belong to a true clump are given a positive label in this extension. The detected regions that were not a clump are given a negative value to clearly identify the sky noise from the diffuse detections. The total number of clumps in this image is stored in the ‘NCLUMPS’ keyword of this extension and printed in verbose output. If the ‘--grownclumps’ option is called, or a value of ‘1’ is given to it in any of the configuration files, then instead of the original clump regions, the grown clumps will be stored in this extension. Note that if there is only one clump (or no clumps) over a detected region, then the whole detected region is given a label of 1. 4. The final sky value on each pixel. See *note Sky value:: for a complete explanation. 5. Similar to the previous mesh but for the standard deviation on each pixel. To inspect NoiseChisel’s output, you can configure SAO DS9 in your Graphic User Interface (GUI) to open NoiseChisel’s output as a multi-extension data cube. This will allow you to flip through the different extensions and visually inspect the results. This process has been described for the GNOME GUI (most common GUI in GNU/Linux operating systems) in *note Viewing multiextension FITS images::.  File: gnuastro.info, Node: MakeCatalog, Next: Match, Prev: NoiseChisel, Up: Data analysis 7.3 MakeCatalog =============== At the lowest level, a dataset (for example an image) is just a collection of values, placed after each other in any number of dimensions (for example an image is a 2D dataset). Each data-element (pixel) just has two properties: its position (relative to the rest) and its value. The entire input dataset (a large image for example) is rarely treated as a singular entity for higher-level analysis(1). You want to know the properties of the scientifically interesting targets that are embedded in it. For example the magnitudes, positions and elliptical properties of the galaxies that are in the image. MakeCatalog is Gnuastro’s program to derive higher-level information for _pre-defined_ regions of a dataset. The role of MakeCatalog in a scientific analysis and the benefits of this model of data-analysis (were detection/identification is separated from measurement) is discussed in Akhlaghi [2016] (https://arxiv.org/abs/1611.06387v1). We strongly recommend reading this short paper for a better understanding of this methodology and use MakeCatalog most effectively. However, that paper cannot undergo any more change, so this manual is the definitive guide. As discussed above, you have to define the regions of a dataset that you are interested in _before_ running MakeCatalog. MakeProfiles currently uses labeled dataset(s) for this job. A labeled dataset for a given input dataset has the size/dimensions as the input, but its pixels have an integer type (see *note Numeric data types::)(2): all pixels with the same label (integers larger and equal to one) are used to generate the requested output columns of MakeCatalog for the row of their labeled value. For example, the flux weighted average position of all the pixels with a label of 42 will be considered as the central position(3) of the 42nd row of the output catalog. Pixels with labels equal to or smaller than zero will be ignored by MakeCatalog. In other words, the number of rows of the output catalog will be determined from the labeled image. The labeled image maybe created with any tool(4). Within Gnuastro you can use these two solutions depending on a-priori/parametric knowledge of the targets you want to study: • When you already know the positions and parametric (for example circular or elliptical) properties of the targets, you can use *note MakeProfiles:: to generate a labeled image from another catalog. This is also known as aperture photometry (the apertures are defined a-priori). • When the shape of your targets cannot be parameterized accurately (for example galaxies), or if you don’t know the number/shape of the targets in the image, you can use Gnuastro’s NoiseChisel program to detect and segment (make labeled images of) the _objects_ and _clumps_ in the input image, see *note NoiseChisel::. * Menu: * Detection and catalog production:: Discussing why/how to treat these separately * Quantifying measurement limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Adding new columns to MakeCatalog:: How to add new columns. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. ---------- Footnotes ---------- (1) In low-level reduction/preparation of a dataset, you do in fact treat a whole image as a single entity. You can derive the over-all properties of all the pixels in a dataset with Gnuastro’s Statistics program (see *note Statistics::) (2) If the program you used to generate the labeled image only outputs floating point types, but you know it only has integer valued pixels that are stored in a floating point container, you can use Gnuastro’s Arithmetic program (see *note Arithmetic::) to change the numerical data type of the image (‘flabel.fits’) to an integer type image (‘label.fits’) with a command like below: ‘$ astarithmetic flabel.fits int32 --output=label.fits’ (3) See *note Measuring elliptical parameters:: for a discussion on this and the derivation of positional parameters. (4) For example, you can even use a graphic user interface image editing tool like the GNU Image Manipulation Program (or GIMP) and use Gnuastro’s ConvertType to convert it to a FITS file.  File: gnuastro.info, Node: Detection and catalog production, Next: Quantifying measurement limits, Prev: MakeCatalog, Up: MakeCatalog 7.3.1 Detection and catalog production -------------------------------------- As discussed above (*note MakeCatalog::), NoiseChisel (Gnuastro’s signal detection tool, see *note NoiseChisel::) does not produce any catalog of the detected objects. However, most other common tools in astronomical data-analysis (for example SExtractor(1)) merge the two processes into one. Gnuastro’s modularized methodology is therefore new to many experienced astronomers and deserves a short review here. Further discussion on the benefits of this methodology can be seen in Akhlaghi [2016] (https://arxiv.org/abs/1611.06387v1). To simplify catalog production from a raw input image in Gnuastro, NoiseChisel’s output (see *note NoiseChisel output::) can be directly fed into MakeCatalog. This is good when no further customization is necessary and you want a fast/simple. But the modular approach taken by Gnuastro has many benefits that will become more apparent as you get more experienced in astronomical data analysis and want to be more creative in using your valuable data for the exciting scientific project you are working on. In short the reasons for this modularity can be classified as below: • Complexity of a monolith: Adding in a catalog functionality to the detector program will add several more steps (and many more options) to its processing that can equally well be done outside of it. This makes following what the program does harder for the users and developers, it can also potentially add many bugs. As an example, if the parameter you want to measure over one profile is not provided by the developers of MakeCatalog. You can simply open this tiny little program and add your desired calculation easily. This process is discussed in *note Adding new columns to MakeCatalog::. However, if making a catalog was part of NoiseChisel, it would require a lot of energy to understand all the steps and internal structures of that large program (the most complex in Gnuastro) in order to add desired parameter in a catalog. • Simplicity/robustness of independent, modular tools: making a catalog is a logically separate process from labeling (detection and segmentation). A user might want to do certain operations on the labeled regions before creating a catalog for them. Another user might want the properties of the same pixels/objects in another image (another filter for example) to measure the colors or SED fittings. Here is an example of doing both: suppose you have images in various broad band filters at various resolutions and orientations. The image of one color will thus not lie exactly on another or even be in the same scale. However, it is imperative that the same pixels be used in measuring the colors of galaxies. To solve the problem, NoiseChisel can be run on the reference image to generate the labeled image. After wards, the labeled image can be warped into the grid of the other color (using *note Warp::). MakeCatalog will then generate the same catalog for both colors (with the different labeled images). It is currently customary to warp the images to the same pixel grid, however, modification of the scientific dataset is very harmful for the data and creates correlated noise. It is much more accurate to do the transformations on the labeled image. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Quantifying measurement limits, Next: Measuring elliptical parameters, Prev: Detection and catalog production, Up: MakeCatalog 7.3.2 Quantifying measurement limits ------------------------------------ No measurement on a real dataset can be perfect: you can only reach a certain level/limit of accuracy. Therefore, a meaningful (scientific) analysis requires an understanding of these limits for the dataset and your analysis tools: different datasets (images in the case of MakeCatalog) have different noise properties and different detection methods (one method/algorith/software that is run with a different set of parameters is considered as a different detection method) will have different abilities to detect or measure certain kinds of signal (astronomical objects) and their properties in an image. Hence, quantifying the detection and measurement limitations with a particular dataset and analysis tool is the most crucial/critical aspect of any high-level analysis. In this section we discuss some of the most general limits that are very important in any astronomical data analysis and how MakeCatalog makes it easy to find them. Depending on the higher-level analysis, there are more tests that must be done, but these are usually necessary in any case. In astronomy, it is common to use the magnitude (a unit-less scale) and physical units, see *note Flux Brightness and magnitude::. Therefore all the measurements discussed here are defined in units of magnitudes. Surface brightness limit (of whole dataset) As we make more observations on one region of the sky, and add the observations into one dataset, we are able to decrease the standard deviation of the noise in each pixel(1). Qualitatively, this decrease manifests its self by making fainter (per pixel) parts of the objects in the image more visible. Technically, this is known as surface brightness. Quantitatively, it increases the Signal to noise ratio, since the signal increases faster than noise with more data. It is very important to have in mind that here, noise is defined per pixel (or in the units of our data measurement), not per object. You can think of the noise as muddy water that is completely covering a flat ground(2) with some regions higher than the others(3) in it. In this analogy, height (from the ground) is _surface brightness_. Let’s assume that in your first observation the muddy water has just been stirred and you can’t see anything through it. As you wait and make more observations, the mud settles down and the _depth_ of the transparent water increases, making the summits of hills visible. As the depth of clear water increases, the parts of the hills with lower heights (less parts with lower surface brightness) can be seen more clearly. The outputs of NoiseChisel include the Sky standard deviation ($\sigma$) on every group of pixels (a mesh) that were calculated from the undetected pixels in that mesh, see *note Tessellation:: and *note NoiseChisel output::. Let’s take $\sigma_m$ as the median $\sigma$ over the successful meshes in the image (prior to interpolation or smoothing). On different instruments pixels have different physical sizes (for example in micro-meters, or spatial angle over the sky), nevertheless, a pixel is our unit of data collection. In other words, while quantifying the noise, the physical or projected size of the pixels is irrelevant. We thus define the Surface brightness limit or _depth_, in units of magnitude/pixel, of a data-set, with zeropoint magnitude $z$, with the $n$th multiple of $\sigma_m$ as (see *note Flux Brightness and magnitude::): $$SB_{\rm Pixel}=-2.5\times\log_{10}{(n\sigma_m)}+z$$ As an example, the XDF survey covers part of the sky that the Hubble space telescope has observed the most (for 85 orbits) and is consequently very small ($\sim4$ arcmin$^2$). On the other hand, the CANDELS survey, is one of the widest multi-color surveys covering several fields (about 720 arcmin$^2$) but its deepest fields have only 9 orbits observation. The depth of the XDF and CANDELS-deep surveys in the near infrared WFC3/F160W filter are respectively 34.40 and 32.45 magnitudes/pixel. In a single orbit image, this same field has a depth of 31.32. Recall that a larger magnitude corresponds to less brightness. The low-level magnitude/pixel measurement above is only useful when all the datasets you want to use belong to one instrument (telescope and camera). However, you will often find yourself using datasets from various instruments with different pixel scales (projected pixel sizes). If we know the pixel scale, we can obtain a more easily comparable surface brightness limit in units of: magnitude/arcsec$^2$. Let’s assume that the dataset has a zeropoint value of $z$, and every pixel is $p$ arcsec$^2$ (so $A/p$ is the number of pixels that cover an area of $A$ arcsec$^2$). If the $n$th multiple of $\sigma_m$ is desired, then the surface brightness (in units of magnitudes per A arcsec$^2$) is(4): $$SB_{\rm Projected}=-2.5\times\log_{10}{\left(n\sigma_m\sqrt{A\over p}\right)+z}$$ Note that this is an extrapolation of the actually measured value of $\sigma_m$ (which was per pixel). So it should be used with extreme care (for example the dataset must have an approximately flat depth). For each detection over the dataset, you can estimate an upper-limit magnitude which actually uses the detection’s area/footprint. It doesn’t extrapolate and even accounts for correlated noise features. Therefore, the upper-limit magnitude is a much better measure of your dataset’s surface brightness limit for each particular object. MakeCatalog will calculate the input dataset’s $SB_{\rm Pixel}$ and $SB_{\rm Projected}$ and write them as comments/meta-data in the output catalog(s). Just note that $SB_{\rm Projected}$ is only calculated if the input has World Coordinate System (WCS). Completeness limit (of each detection) As the surface brightness of the objects decreases, the ability to detect them will also decrease. An important statistic is thus the fraction of objects of similar morphology and brightness that will be identified with our detection algorithm/parameters in the given image. This fraction is known as completeness. For brighter objects, completeness is 1: all bright objects that might exist over the image will be detected. However, as we go to lower surface brightness objects, we fail to detect some and gradually we are not able to detect anything any more. For a given profile, the magnitude where the completeness drops below a certain level usually above $90\%$ is known as the completeness limit. Another important parameter in measuring completeness is purity: the fraction of true detections to all true detections. In effect purity is the measure of contamination by false detections: the higher the purity, the lower the contamination. Completeness and purity are anti-correlated: if we can allow a large number of false detections (that we might be able to remove by other means), we can significantly increase the completeness limit. One traditional way to measure the completeness and purity of a given sample is by embedding mock profiles in regions of the image with no detection. However in such a study we must be really careful to choose model profiles as similar to the target of interest as possible. Magnitude measurement error (of each detection) Any measurement has an error and this includes the derived magnitude for an object. Note that this value is only meaningful when the object’s magnitude is brighter than the upper-limit magnitude (see the next items in this list). As discussed in *note Flux Brightness and magnitude::, the magnitude ($M$) of an object with brightness $B$ and Zeropoint magnitude $z$ can be written as: $$M=-2.5\log_{10}(B)+z$$ Calculating the derivative with respect to $B$, we get: $${dM\over dB} = {-2.5\over {B\times ln(10)}}$$ From the Tailor series ($\Delta{M}=dM/dB\times\Delta{B}$), we can write: $$\Delta{M} = \left|{-2.5\over ln(10)}\right|\times{\Delta{B}\over{B}}$$ But, $\Delta{B}/B$ is just the inverse of the Signal-to-noise ratio ($S/N$), so we can write the error in magnitude in terms of the signal-to-noise ratio: $$\Delta{M} = {2.5\over{S/N\times ln(10)}} $$ MakeCatalog uses this relation to estimate the magnitude errors. The signal-to-noise ratio is calculated in different ways for clumps and objects (see Akhlaghi and Ichikawa [2015] (https://arxiv.org/abs/1505.01664)), but this single equation can be used to estimate the measured magnitude error afterwards for any type of target. Upper limit magnitude (of each detection) Due to the noisy nature of data, it is possible to get arbitrarily low values for a faint object’s brightness (or arbitrarily high magnitudes). Given the scatter caused by the noise, such small values are meaningless: another similar depth observation will give a radically different value. This problem is most common when you use one image/filter to generate target labels (which specify which pixels belong to which object, see *note NoiseChisel output:: and *note MakeCatalog::) and another image/filter to generate a catalog for measuring colors. The object might not be visible in the filter used for the latter image, or the image _depth_ (see above) might be much shallower. So you will get unreasonably faint magnitudes. For example when the depth of the image is 32 magnitudes, a measurement that gives a magnitude of 36 for a $\sim100$ pixel object is clearly unreliable. In another similar depth image, we might measure a magnitude of 30 for it, and yet another might give 33. Furthermore, due to the noise scatter so close to the depth of the data-set, the total brightness might actually get measured as a negative value, so no magnitude can be defined (recall that a magnitude is a base-10 logarithm). Using such unreliable measurements will directly affect our analysis, so we must not use them. However, all is not lost! Given our limited depth, there is one thing we can deduce about the object’s magnitude: we can say that if something actually exists here (possibly buried deep under the noise), it must have a magnitude that is fainter than an _upper limit magnitude_. To find this upper limit magnitude, we place the object’s footprint (segmentation map) over random parts of the image where there are no detections, so we only have pure (possibly correlated) noise and undetected objects. Doing this a large number of times will give us a distribution of brightness values. The standard deviation ($\sigma$) of that distribution can be used to quantify the upper limit magnitude. Traditionally, faint/small object photometry was done using fixed circular apertures (for example with a diameter of $N$ arc-seconds). In this way, the upper limit was like the depth discussed above: one value for the whole image. But with the much more advanced hardware and software of today, we can make customized segmentation maps for each object. The number of pixels (are of the object) used directly affects the final distribution and thus magnitude. Also the image correlated noise might actually create certain patters, so the shape of the object can also affect the result. So in MakeCatalog, the upper limit magnitude is found for each object in the image separately. Not one value for the whole image. ---------- Footnotes ---------- (1) This is true for any noisy data, not just astronomical images. (2) The ground is the sky value in this analogy, see *note Sky value::. Note that this analogy only holds for a flat sky value across the surface of the image or ground. (3) The peaks are the brightest parts of astronomical objects in this analogy. (4) If we have $N$ datasets, each with noise $\sigma$, the noise of a combined dataset will increase as $\sqrt{N}\sigma$.  File: gnuastro.info, Node: Measuring elliptical parameters, Next: Adding new columns to MakeCatalog, Prev: Quantifying measurement limits, Up: MakeCatalog 7.3.3 Measuring elliptical parameters ------------------------------------- The shape or morphology of a target is one of the most commonly desired parameters of a target. Here, we will review the derivation of the most basic/simple morphological parameters: the elliptical parameters for a set of labeled pixels. The elliptical parameters are: the (semi-)major axis, the (semi-)minor axis and the position angle along with the central position of the profile. The derivations below follow the SExtractor manual derivations with some added explanations for easier reading. Let’s begin with one dimension for simplicity: Assume we have a set of $N$ values $B_i$ (keeping the spatial distribution of brightness for example), each at position $x_i$. The simplest parameter we can define is the geometric center of the object ($x_g$) (ignoring the brightness values): $x_g=(\sum_ix_i)/N$. _Moments_ are defined to incorporate both the value (brightness) and position of the data. The first moment can be written as: $$\overline{x}={\sum_iB_ix_i \over \sum_iB_i}$$ This is essentially the weighted (by $B_i$) mean position. The geometric center ($x_g$, defined above) is a special case of this with all $B_i=1$. The second moment is essentially the variance of the distribution: $$\overline{x^2}\equiv{\sum_iB_i(x_i-\overline{x})^2 \over \sum_iB_i} = {\sum_iB_ix_i^2 \over \sum_iB_i} - 2\overline{x}{\sum_iB_ix_i\over\sum_iB_i} + \overline{x}^2 ={\sum_iB_ix_i^2 \over \sum_iB_i} - \overline{x}^2$$ The last step was done from the definition of $\overline{x}$. Hence, the square root of $\overline{x^2}$ is the spatial standard deviation (along the one-dimension) of this particular brightness distribution ($B_i$). Crudely (or qualitatively), you can think of its square root as the distance (from $\overline{x}$) which contains a specific amount of the flux (depending on the $B_i$ distribution). Similar to the first moment, the geometric second moment can be found by setting all $B_i=1$. So while the first moment quantified the position of the brightness distribution, the second moment quantifies how that brightness is dispersed about the first moment. In other words, it quantifies how “sharp†the object’s image is. Before continuing to two dimensions and the derivation of the elliptical parameters, let’s pause for an important implementation technicality. You can ignore this paragraph and the next two if you don’t want to implement these concepts. The basic definition (first definition of $\overline{x^2}$ above) can be used without any major problem. However, using this fraction requires two runs over the data: one run to find $\overline{x}$ and another run to find $\overline{x^2}$ from $\overline{x}$, this can be slow. The advantage of the last fraction above, is that we can estimate both the first and second moments in one run (since the $-\overline{x}^2$ term can easily be added later). The logarithmic nature of floating point number digitization creates a complication however: suppose the object is located between pixels 10000 and 10020. Hence the target’s pixels are only distributed over 20 pixels (with a standard deviation $<20$), while the mean has a value of $\sim10000$. The $\sum_iB_i^2x_i^2$ will go to very very large values while the individual pixel differences will be orders of magnitude smaller. This will lower the accuracy of our calculation due to the limited accuracy of floating point operations. The variance only depends on the distance of each point from the mean, so we can shift all position by a constant/arbitrary $K$ which is much closer to the mean: $\overline{x-K}=\overline{x}-K$. Hence we can calculate the second order moment using: $$\overline{x^2}={\sum_iB_i(x_i-K)^2 \over \sum_iB_i} - (\overline{x}-K)^2 $$ The closer $K$ is to $\overline{x}$, the better (the sums of squares will involve smaller numbers), as long as $K$ is within the object limits (in the example above: $10000\leq{K}\leq10020$), the floating point error induced in our calculation will be negligible. For the most simplest implementation, MakeCatalog takes $K$ to be the smallest position of the object in each dimension. Since $K$ is arbitrary and an implementation/technical detail, we will ignore it for the remainder of this discussion. In two dimensions, the mean and variances can be written as: $$\overline{x}={\sum_iB_ix_i\over B_i}, \quad \overline{x^2}={\sum_iB_ix_i^2 \over \sum_iB_i} - \overline{x}^2$$ $$\overline{y}={\sum_iB_iy_i\over B_i}, \quad \overline{y^2}={\sum_iB_iy_i^2 \over \sum_iB_i} - \overline{y}^2$$ $$\quad\quad\quad\quad\quad\quad\quad\quad\quad \overline{xy}={\sum_iB_ix_iy_i \over \sum_iB_i} - \overline{x}\times\overline{y}$$ If an elliptical profile’s major axis exactly lies along the $x$ axis, then $\overline{x^2}$ will be directly proportional with the profile’s major axis, $\overline{y^2}$ with its minor axis and $\overline{xy}=0$. However, in reality we are not that lucky and (assuming galaxies can be parameterized as an ellipse) the major axis of galaxies can be in any direction on the image (in fact this is one of the core principles behind weak-lensing by shear estimation). So the purpose of the remainder of this section is to define a strategy to measure the position angle and axis ratio of some randomly positioned ellipses in an image, using the raw second moments that we have calculated above in our image coordinates. Let’s assume we have rotated the galaxy by $\theta$, the new second order moments are: $$\overline{x_\theta^2} = \overline{x^2}\cos^2\theta + \overline{y^2}\sin^2\theta - 2\overline{xy}\cos\theta\sin\theta $$ $$\overline{y_\theta^2} = \overline{x^2}\sin^2\theta + \overline{y^2}\cos^2\theta + 2\overline{xy}\cos\theta\sin\theta$$ $$\overline{xy_\theta} = \overline{x^2}\cos\theta\sin\theta - \overline{y^2}\cos\theta\sin\theta + \overline{xy}(\cos^2\theta-\sin^2\theta)$$ The best $\theta$ ($\theta_0$, where major axis lies along the $x_\theta$ axis) can be found by: $$\left.{\partial \overline{x_\theta^2} \over \partial \theta}\right|_{\theta_0}=0$$ Taking the derivative, we get: $$2\cos\theta_0\sin\theta_0(\overline{y^2}-\overline{x^2}) + 2(\cos^2\theta_0-\sin^2\theta_0)\overline{xy}=0$$ When $\overline{x^2}\neq\overline{y^2}$, we can write: $$\tan2\theta_0 = 2{\overline{xy} \over \overline{x^2}-\overline{y^2}}.$$ MakeCatalog uses the standard C math library’s ‘atan2’ function to estimate $\theta_0$, which we define as the position angle of the ellipse. To recall, this is the angle of the major axis of the ellipse with the $x$ axis. By definition, when the elliptical profile is rotated by $\theta_0$, then $\overline{xy_{\theta_0}}=0$, $\overline{x_{\theta_0}^2}$ will be the extent of the maximum variance and $\overline{y_{\theta_0}^2}$ the extent of the minimum variance (which are perpendicular for an ellipse). Replacing $\theta_0$ in the equations above for $\overline{x_\theta}$ and $\overline{y_\theta}$, we can get the semi-major ($A$) and semi-minor ($B$) lengths: $$A^2\equiv\overline{x_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} + \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}$$ $$B^2\equiv\overline{y_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} - \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}$$ As a summary, it is important to remember that the units of $A$ and $B$ are in pixels (the standard deviation of a positional distribution) and that they represent the spatial light distribution of the object in both image dimensions (rotated by $\theta_0$). When the object cannot be represented as an ellipse, this interpretation breaks down: $\overline{xy_{\theta_0}}\neq0$ and $\overline{y_{\theta_0}^2}$ will not be the direction of minimum variance.  File: gnuastro.info, Node: Adding new columns to MakeCatalog, Next: Invoking astmkcatalog, Prev: Measuring elliptical parameters, Up: MakeCatalog 7.3.4 Adding new columns to MakeCatalog --------------------------------------- MakeCatalog is designed to allow easy addition of different measurements over a labeled image (see Akhlaghi [2016] (https://arxiv.org/abs/1611.06387v1)). A check-list style description of necessary steps to do that is described in this section. The common development characteristics of MakeCatalog and other Gnuastro programs is explained in *note Developing::. We strongly encourage you to have a look at that chapter to greatly simplify your navigation in the code. After adding and testing your column, you are most welcome (and encouraged) to share it with us so we can add to the next release of Gnuastro for everyone else to also benefit from your efforts. MakeCatalog will first pass over each label’s pixels two times and do necessary raw/internal calculations. Once the passes are done, it will use the raw information for filling the final catalog’s columns. In the first pass it will gather mainly object information and in the second run, it will mainly focus on the clumps, or any other measurement that needs an output from the first pass. These two passes are designed to be raw summations: no extra processing. This will allow parallel processing and simplicity/clarity. So if your new calculation, needs new raw information from the pixels, then you will need to also modify the respective ‘mkcatalog_first_pass’ and ‘mkcatalog_second_pass’ functions (both in ‘bin/mkcatalog/mkcatalog.c’) and define new raw table columns in ‘main.h’ (hopefully the comments in the code are clear enough). In all these different places, the final columns are sorted in the same order (same order as *note Invoking astmkcatalog::). This allows a particular column/option to be easily found in all steps. Therefore in adding your new option, be sure to keep it in the same relative place in the list in all the separate places (it doesn’t necessarily have to be in the end), and near conceptually similar options. ‘main.h’ The ‘objectcols’ and ‘clumpcols’ enumerated variables (‘enum’) define the raw/internal calculation columns. If your new column requires new raw calculations, add a row to the respective list. If your calculation requires any other settings parameters, you should add a variable to the ‘mkcatalogparams’ structure. ‘ui.h’ The ‘option_keys_enum’ associates a unique value for each option to MakeProfiles. The options that have a short option version, the single character short comment is used for the value. Those that don’t have a short option version, get a large integer automatically. You should add a variable here to identify your desired column. ‘args.h’ This file specifies all the parameters for the GNU C library, Argp structure that is in charge of reading the user’s options. To define your new column, just copy an existing set of parameters and change the first, second and 5th values (the only ones that differ between all the columns), you should use the macro you defined in ‘ui.h’ here. ‘ui.c’ If your column includes any particular settings (you added a variable to the ‘mkcatalogparams’ structure in ‘main.h’), you should do the sanity checks and preparations for it here. Otherwise, you can ignore this file. ‘columns.c’ This file will contain the main definition and high-level calculation of your new column through the ‘columns_define_alloc’ and ‘columns_fill’ functions. In the first, you specify the basic information about the column: its name, units, comments, type (see *note Numeric data types::) and how it should be printed if the output is a text file. You should also specify the raw/internal columns that are necessary for this column here as the many existing examples show. Through the types for objects and rows, you can specify if this column is only for clumps, objects or both. The second main function (‘columns_fill’) writes the final value into the appropriate column for each object and clump. As you can see in the many existing examples, you can define your processing on the raw/internal calculations here and save them in the output. ‘mkcatalog.c’ As described before, this file contains the two main MakeCatalog work-horses: ‘mkcatalog_first_pass’ and ‘mkcatalog_second_pass’, their names are descriptive enough and their internals are also clear and heavily commented.  File: gnuastro.info, Node: Invoking astmkcatalog, Prev: Adding new columns to MakeCatalog, Up: MakeCatalog 7.3.5 Invoking MakeCatalog -------------------------- MakeCatalog will make a catalog from an input image and at least on labeled image. The executable name is ‘astmkcatalog’ with the following general template $ astmkcatalog [OPTION ...] InputImage.fits One line examples: ## Create catalog with RA, Dec, Magnitude and Magnitude error, ## `input.fits' is NoiseChisel's output: $ astmkcatalog --ra --dec --magnitude --magnitudeerr input.fits ## Same catalog as above (using short options): $ asmkcatalog -rdmG input.fits ## Write the catalog to a FITS table: $ astmkcatalog -mpQ --output=cat.fits input_labeled.fits ## Read the columns to create from `columns.conf': $ astmkcatalog --config=columns.conf input_labeled.fits ## Use different images for the objects and clumps inputs: $ astmkcatalog --objectsfile=K_labeled.fits --objectshdu=1 \ --clumpsfile=K_labeled.fits --clumpshdu=2 i_band.fits If MakeCatalog is to do processing, an input image should be provided with the recognized extensions as input data, see *note Arguments::. The options described in this section are those that are only particular to MakeProfiles. For operations that MakeProfiles shares with other programs (mainly involving input/output or general processing steps), see *note Common options::. Also see *note Common program behavior:: for some general characteristics of all Gnuastro programs including MakeCatalog. MakeCatalog needs 4 (or 5) images as input. These images can be separate extensions in one file (NoiseChisel’s default output), or each can have its own file and its own extension. See *note NoiseChisel output:: for the list. The clump labels image is not mandatory (when no clump catalog is required, for example in aperture photometry). When inspecting the object labels image, MakeProfiles will look for a ‘WCLUMPS’ (short for with-clumps) header keyword. If that keyword is present and has a value of ‘yes’, ‘1’, or ‘y’ (case insensitive) then a clump image must also be provided and a clump catalog will be made. When ‘WCLUMPS’ isn’t present or has any other value, only an object catalog will be created and all clump related options/columns will be ignored. For example, if you only need an object catalog from NoiseChisel’s output, you can use Gnuastro’s Fits program (see *note Fits::) to modify or remove the ‘WCLUMPS’ keyword in the objects HDU, then run MakeCatalog on it. Another example can be aperture photometry: let’s assume you have made your labeled image (defining the apertures) with MakeProfiles. Clumps are not defined in this context, so besides the input and labeled image, you only need NoiseChisel’s Sky and Sky standard deviation images (run NoiseChisel with the ‘--onlydetection’ option). Since MakeProfile’s output doesn’t contain the ‘WCLUMPS’ keyword, you just have to specify your labeled image with the ‘--objectsfile’ option and also set its HDU. Note that labeled images have to be an integer type. Therefore, if you are using MakeProfiles to define the apertures/labels, you can use its ‘--type=int32’ for example, see *note Input output options:: and *note Numeric data types::. When a clump catalog is also desired, two catalogs will be made: one for the objects (suffixed with ‘_o.txt’ or ‘_o.fits’) and another for the clumps (suffixed with ‘_c.txt’ or ‘_c.fits’). Therefore if any value is given to the ‘--output’ option, MakeCatalogs will replace these two suffixes with any existing suffix in the given value. If no output value is given, MakeCatalog will use the input name, see *note Automatic output::. The format of the output table is specified with the ‘--tableformat’ option, see *note Input output options::. When MakeCatalog is run on multiple threads, the clumps catalog rows will not be sorted by object since each object is processed independently by one thread and threaded applications are asynchronous. The clumps in each object will be sorted based on their labels, but you will find lower-index objects come after higher-index ones (especially if they have more clumps and thus take more time). If the order is very important for you, you can run the following command to sort the rows by object ID (and clump ID with each object): $ awk '!/^#/' out_c.txt | sort -g -k1,1 -k2,2 * Menu: * MakeCatalog input files:: Specifying the different input files. * MakeCatalog general settings:: Options for general column settings. * Upper-limit magnitude settings:: Necessary to define upper-limit magnitudes. * MakeCatalog output columns:: How to specify the columns in the output.  File: gnuastro.info, Node: MakeCatalog input files, Next: MakeCatalog general settings, Prev: Invoking astmkcatalog, Up: Invoking astmkcatalog 7.3.5.1 MakeCatalog input files ............................... MakeCatalog needs multiple images as input: a values image, one (or two) labeled images and Sky and Sky standard deviation images. The options described in this section allow you to identify them. If you use the default output of NoiseChisel (see *note NoiseChisel output::) you don’t have to worry about any of these options and just give NoiseChisel’s output file to MakeCatalog as described in *note Invoking astmkcatalog::. ‘-O STR’ ‘--objectsfile=STR’ The file name of the object labels image, if the image is in another extension of the input file, calling this option is not mandatory, just specify the extension/HDU with the ‘--objectshdu’ option. ‘--objectshdu=STR’ The HDU/extension of the object labels image. Only pixels with values above zero will be considered. The objects label image has to be an integer data type (see *note Numeric data types::) and only pixels with a value larger than zero will be used. If this extension contains the ‘WCLUMPS’ keyword with a value of ‘yes’, ‘1’, or ‘y’ (not case sensitive), then MakeCatalog will also build a clumps catalog, see *note Invoking astmkcatalog::. ‘-C STR’ ‘--clumpsfile=STR’ Similar to ‘--objlabs’ but for the labels of the clumps. This is only necessary if the image containing clump labels is not in the input file and the objects image has a ‘WCLUMPS’ keyword, see ‘--objectshdu’. ‘--clumpshdu=STR’ The HDU/extension of the object labels image. Only pixels with values above zero will be considered. The objects label image has to be an integer data type (see *note Numeric data types::) and only pixels with a value larger than zero will be used. ‘-s STR’ ‘--skyfile=STR’ File name of an image keeping the Sky value for each pixel. ‘--skyhdu=STR’ The HDU of the Sky value image. ‘-t STR’ ‘--stdfile=STR’ File name of image keeping the Sky value standard deviation for each pixel. ‘--stdhdu=STR’ The HDU of the Sky value standard deviation image.  File: gnuastro.info, Node: MakeCatalog general settings, Next: Upper-limit magnitude settings, Prev: MakeCatalog input files, Up: Invoking astmkcatalog 7.3.5.2 MakeCatalog general settings .................................... Some of the columns require particular settings (for example the zero point magnitude for measuring magnitudes), the options in this section can be used for such configurations. ‘-z FLT’ ‘--zeropoint=FLT’ The zero point magnitude for the input image, see *note Flux Brightness and magnitude::. ‘-E’ ‘--skysubtracted’ If the image has already been sky subtracted by another program, then you need to notify MakeCatalog through this option. Note that this is only relevant when the Signal to noise ratio is to be calculated. ‘-T FLT’ ‘--threshold=FLT’ For all the columns, only consider pixels that are above a given relative threshold. Symbolizing the value of this option as $T$, the Sky for a pixel at $(i,j)$ with $\mu_{ij}$ and its Standard deviation with $\sigma_{ij}$, that pixel will only be used if its value ($B_{ij}$) satisfies this condition: $B_{ij}>\mu_{ij}+{T}\sigma_{ij}$. The only calculations that will not be affected are is the average river values (‘--riverave’), since they are used as a reference. A commented row will be added in the header of the output catalog that will print the given value, since this is a very important issue, it starts with ‘**IMPORTANT**’. NoiseChisel will detect very diffuse signal which is useful in most cases where the aggregate properties of the detections are desired, since there is signal there (with the desired certainty). However, in some cases, only the properties of the peaks of the objects/clumps are desired, for example in attempting to separate stars from galaxies, the peaks are the major target and the diffuse regions only act to complicate the separation. With this option, MakeCatalog will simply ignore any pixel below the relative threshold. This option is not mandatory, so if it isn’t given (after reading the command-line and all configuration files, see *note Configuration files::), MakeCatalog will still operate. However, if it has a value in any lower-level configuration file and you want to ignore that value for this particular run or in a higher-level configuration file, then set it to NaN, for example ‘--threshold=nan’. Gnuastro uses the C library’s ‘strtod’ function to read floats, which is not case-sensitive in reading NaN values. But to be consistent, it is good practice to only use ‘nan’. ‘--nsigmag=FLT’ The median standard deviation (from the standard deviation image) will be multiplied by the value to this option and its magnitude will be reported in the comments of the output catalog. This value is a per-pixel value, not per object/clump and is not found over an area or aperture, like the common $5\sigma$ values that are commonly reported as a measure of depth or the upper-limit measurements (see *note Quantifying measurement limits::).  File: gnuastro.info, Node: Upper-limit magnitude settings, Next: MakeCatalog output columns, Prev: MakeCatalog general settings, Up: Invoking astmkcatalog 7.3.5.3 Upper-limit magnitude settings ...................................... The upper limit magnitude was discussed in *note Quantifying measurement limits::. Unlike other measured values/columns in MakeCatalog, the upper limit magnitude needs several defined parameters which are discussed here. All the upper limit magnitude specific options start with ‘up’ for upper-limit, except for ‘--envseed’ that is also present in other programs and is general for any job requiring random number generation (see *note Generating random numbers::). One very important consideration in Gnuastro is reproducibility. Therefore, the values to all of these parameters along with others (like the random number generator type and seed) are also reported in the comments of the final catalog when the upper limit magnitude column is desired. The random seed that is used to define the random positionings for each object or clump is unique and set based on the given seed, the total number of objects and clumps and also the labels of the clumps and objects. So with identical inputs, an identical upper-limit magnitude will be found. But even if the ordering of the object/clump labels differs (and the seed is the same) the result will not be the same. MakeCatalog will randomly place the object/clump footprint over the image and when the footprint doesn’t fall on any object or masked region (see ‘--upmaskfile’) it will be used until the desired number (‘--upnum’) of samples are found to estimate the distribution’s standard deviation (see *note Quantifying measurement limits::). Otherwise it will be ignored and another random position will be generated. But when the profile is very large or the image is significantly covered by detections, it might not be possible to find the desired number of samplings. MakeProfiles will continue searching until 50 times the value given to ‘--upnum’. If ‘--upnum’ good samples cannot be found until this limit, it will set the upper-limit magnitude for that object to NaN (blank). MakeCatalog will also print a warning if the range of positions available for the labeled region is smaller than double the size of the region. In such cases, the limited range of random positions can artificially decrease the standard deviation of the final distribution. ‘--upmaskfile=STR’ File name of mask image to use for upper-limit calculation. In some cases (especially when doing matched photometry), the object labels specified in the main input and mask image might not be adequate. In other words they do not necessarily have to cover _all_ detected objects: the user might have selected only a few of the objects in their labeled image. This option can be used to ignore regions in the image in these situations when estimating the upper-limit magnitude. All the non-zero pixels of the image specified by this option (in the ‘--upmaskhdu’ extension) will be ignored in the upper-limit magnitude measurements. For example, when you are using labels from another image, you can give NoiseChisel’s objects image output for this image as the value to this option. In this way, you can be sure that regions with data do not harm your distribution. See *note Quantifying measurement limits:: for more on the upper limit magnitude. ‘--upmaskhdu=STR’ The extension in the file specified by ‘--upmask’. ‘--upnum=INT’ The number of random samples to take for all the objects. A larger value to this option will give a more accurate result (asymptotically), but it will also slow down the process. When a randomly positioned sample overlaps with a detected/masked pixel it is not counted and another random position is found until the object completely lies over an undetected region. So you can be sure that for each object, this many samples over undetected objects are made. See the upper limit magnitude discussion in *note Quantifying measurement limits:: for more. ‘--uprange=INT,INT’ The range/width of the region (in pixels) to do random sampling along each dimension of the input image around each object’s position. This is not a mandatory option and if not given (or given a value of zero in a dimension), the full possible range of the dataset along that dimension will be used. This is useful when the noise properties of the dataset vary gradually. In such cases, using the full range of the input dataset is going to bias the result. However, note that decreasing the the range of available positions too much will also artificially decrease the standard deviation of the final distribution (and thus bias the upper-limit measurement). ‘--envseed’ Read the random number generator type and seed value from the environment (see *note Generating random numbers::). Random numbers are used in calculating the random positions of different samples of each object. ‘--upsigmaclip=FLT,FLT’ The raw distribution of random values will not be used to find the upper-limit magnitude, it will first be $\sigma$-clipped (see *note Sigma clipping::) to avoid outliers in the distribution (mainly the faint undetected wings of bright/large objects in the image). This option takes two values: the first is the multiple of $\sigma$, and the second is the termination criteria. If the latter is larger than 1, it is read as an integer number and will be the number of times to clip. If it is smaller than 1, it is interpretted as the tolerance level to stop clipping. See *note Sigma clipping:: for a complete explanation. ‘--upnsigma=FLT’ The multiple of the final ($\sigma$-clipped) standard deviation (or $\sigma$) used to measure the upper-limit brightness or magnitude.  File: gnuastro.info, Node: MakeCatalog output columns, Prev: Upper-limit magnitude settings, Up: Invoking astmkcatalog 7.3.5.4 MakeCatalog output columns .................................. The final group of options particular to MakeCatalog are those that specify which columns should be written into the final output table. For each column there is an option, if it has been called on the command line or in any of the configuration files, it will included as a column in the output catalog in the same order (see *note Configuration file precedence::). Some of the columns apply to both objects and clumps and some are particular to only one of them. The latter cases are explicitly marked with [Objects] or [Clumps] to specify the catalog they will be placed in. ‘--i’ ‘--ids’ This is a unique option which can add multiple columns to the final catalog(s). Calling this option will put the object IDs (‘--objid’) in the objects catalog and host-object-ID (‘--hostobjid’) and ID-in-host-object (‘--idinhostobj’) into the clumps catalog. Hence if only object catalogs are required, it has the same effect as ‘--objid’. ‘--objid’ [Objects] ID of this object. ‘-j’ ‘--hostobjid’ [Clumps] The ID of the object which hosts this clump. ‘--idinhostobj’ [Clumps] The ID of this clump in its host object. ‘-C’ ‘--numclumps’ [Objects] The number of clumps in this object. ‘-a’ ‘--area’ The raw area (number of pixels) in any clump or object independent of what pixel it lies over (if it is NaN/blank or unused for example). ‘--clumpsarea’ [Objects] The total area of all the clumps in this object. ‘--weightarea’ The area (number of pixels) used in the flux weighted position calculations. ‘-x’ ‘--x’ The flux weighted center of all objects and clumps along the first FITS axis (horizontal when viewed in SAO ds9), see $\overline{x}$ in *note Measuring elliptical parameters::. The weight has to have a positive value (pixel value larger than the Sky value) to be meaningful! Specially when doing matched photometry, this might not happen: no pixel value might be above the Sky value. For such detections, the geometric center will be reported in this column (see ‘--geox’). You can use ‘--weightarea’ to see which was used. ‘-y’ ‘--y’ The flux weighted center of all objects and clumps along the second FITS axis (vertical when viewed in SAO ds9). See ‘--x’. ‘--geox’ The geometric center of all objects and clumps along the first FITS axis axis. The geometric center is the average pixel positions irrespective of their pixel values. ‘--geoy’ The geometric center of all objects and clumps along the second FITS axis axis, see ‘--geox’. ‘--clumpsx’ [Objects] The flux weighted center of all the clumps in this object along the first FITS axis. See ‘--x’. ‘--clumpsy’ [Objects] The flux weighted center of all the clumps in this object along the second FITS axis. See ‘--x’. ‘--clumpsgeox’ [Objects] The geometric center of all the clumps in this object along the first FITS axis. See ‘--geox’. ‘--clumpsgeoy’ [Objects] The geometric center of all the clumps in this object along the second FITS axis. See ‘--geox’. ‘-r’ ‘--ra’ Flux weighted right ascension of all objects or clumps, see ‘--x’. This is just an alias for one of the lower-level ‘--w1’ or ‘--w2’ options. Using the FITS WCS keywords (‘CTYPE’), MakeCatalog will determine which axis corresponds to the right ascension. If no ‘CTYPE’ keywords start with ‘RA’, an error will be printed when requesting this column and MakeCatalog will abort. ‘-d’ ‘--dec’ Flux weighted declination of all objects or clumps, see ‘--x’. This is just an alias for one of the lower-level ‘--w1’ or ‘--w2’ options. Using the FITS WCS keywords (‘CTYPE’), MakeCatalog will determine which axis corresponds to the declination. If no ‘CTYPE’ keywords start with ‘DEC’, an error will be printed when requesting this column and MakeCatalog will abort. ‘--w1’ Flux weighted first WCS axis of all objects or clumps, see ‘--x’. The first WCS axis is commonly used as right ascension in images. ‘--w2’ Flux weighted second WCS axis of all objects or clumps, see ‘--x’. The second WCS axis is commonly used as declination in images. ‘--geow1’ Geometric center in first WCS axis of all objects or clumps, see ‘--geox’. The first WCS axis is commonly used as right ascension in images. ‘--geow2’ Geometric center in second WCS axis of all objects or clumps, see ‘--geox’. The second WCS axis is commonly used as declination in images. ‘--clumpsw1’ [Objects] Flux weighted center in first WCS axis of all clumps in this object, see ‘--x’. The first WCS axis is commonly used as right ascension in images. ‘--clumpsw2’ [Objects] Flux weighted declination of all clumps in this object, see ‘--x’. The second WCS axis is commonly used as declination in images. ‘--clumpsgeow1’ [Objects] Geometric center right ascension of all clumps in this object, see ‘--geox’. The first WCS axis is commonly used as right ascension in images. ‘--clumpsgeow2’ [Objects] Geometric center declination of all clumps in this object, see ‘--geox’. The second WCS axis is commonly used as declination in images. ‘-b’ ‘--brightness’ The brightness (sum of all pixel values), see *note Flux Brightness and magnitude::. For clumps, the ambient brightness (flux of river pixels around the clump multiplied by the area of the clump) is removed, see ‘--riverflux’. So the sum of clump brightnesses in the clump catalog will be smaller than the total clump brightness in the ‘--clumpbrightness’ column of the objects catalog. If no usable pixels (blank or below the threshold) are present over the clump or object, the stored value will be NaN (note that zero is meaningful). ‘--clumpbrightness’ [Objects] The total brightness of the clumps within an object. This is simply the sum of the pixels associated with clumps in the object. If no usable pixels (blank or below the threshold) are present over the clump or object, the stored value will be NaN, because zero (note that zero is meaningful). ‘--noriverbrightness’ [Clumps] The Sky (not river) subtracted clump brightness. By definition, for the clumps, the average brightness of the rivers surrounding it are subtracted from it for a first order accounting for contamination by neighbors. In cases where you will be calculating the flux brightness difference later (one example below) the contamination will be (mostly) removed at that stage, which is why this column was added. One example might be this: you want to know the change in the clump flux as a function of threshold (see ‘--threshold’). So you will make two catalogs (each having this column but with different thresholds) and then subtract the lower threshold catalog (higher brightness) from the higher threshold catalog (lower brightness). The effect is most visible when the rivers have a high average signal-to-noise ratio. The removed contribution from the pixels below the threshold will be less than the river pixels. Therefore the river-subtracted brightness (‘--brightness’) for the thresholded catalog for such clumps will be larger than the brightness with no threshold! If no usable pixels (blank or below the possibly given threshold) are present over the clump or object, the stored value will be NaN (note that zero is meaningful). ‘-m’ ‘--magnitude’ The magnitude of clumps or objects, see ‘--brightness’. ‘-e’ ‘--magnitudeerr’ The magnitude error of clumps or objects. The magnitude error is calculated from the signal-to-noise ratio (see ‘--sn’ and *note Quantifying measurement limits::). Note that until now this error assumes un-correlated pixel values and also does not include the error in estimating the aperture (or error in generating the labeled image). For now these factors have to be found by other means. Task 14124 (https://savannah.gnu.org/task/index.php?14124) has been defined for work on adding these sources of error too. ‘--clumpsmagnitude’ [Objects] The magnitude of all clumps in this object, see ‘--clumpbrightness’. ‘--upperlimit’ The upper limit value (in units of the input image) for this object or clump. See *note Quantifying measurement limits:: and *note Upper-limit magnitude settings:: for a complete explanation. This is very important for the fainter and smaller objects in the image where the measured magnitudes are not reliable. ‘--upperlimitmag’ The upper limit magnitude for this object or clump. See *note Quantifying measurement limits:: and *note Upper-limit magnitude settings:: for a complete explanation. This is very important for the fainter and smaller objects in the image where the measured magnitudes are not reliable. ‘--riverave’ [Clumps] The average brightness of the river pixels around this clump. River pixels were defined in Akhlaghi and Ichikawa 2015. In short they are the pixels immediately outside of the clumps. This value is used internally to find the brightness (or magnitude) and signal to noise ratio of the clumps. It can generally also be used as a scale to gauge the base (ambient) flux surrounding the clump. In case there was no river pixels, then this column will have the value of the Sky under the clump. So note that this value is _not_ sky subtracted. ‘--rivernum’ [Clumps] The number of river pixels around this clump, see ‘--riverflux’. ‘-n’ ‘--sn’ The Signal to noise ratio (S/N) of all clumps or objects. See Akhlaghi and Ichikawa (2015) for the exact equations used. ‘--sky’ The sky flux (per pixel) value under this object or clump. This is actually the mean value of all the pixels in the sky image that lie on the same position as the object or clump. ‘--std’ The sky value standard deviation (per pixel) for this clump or object. Like ‘--sky’, this is the average of the values in the input sky standard deviation image pixels that lie over this object. ‘-A’ ‘--semimajor’ The pixel-value weighted semi-major axis of the profile (assuming it is an ellipse) in units of pixels. See *note Measuring elliptical parameters::. ‘-B’ ‘--semiminor’ The pixel-value weighted semi-minor axis of the profile (assuming it is an ellipse) in units of pixels. See *note Measuring elliptical parameters::. ‘-p’ ‘--positionangle’ The pixel-value weighted angle of the semi-major axis with the first FITS axis in degrees. See *note Measuring elliptical parameters::. ‘--geosemimajor’ The geometric (ignoring pixel values) semi-major axis of the profile, assuming it is an ellipse. ‘--geosemiminor’ The geometric (ignoring pixel values) semi-minor axis of the profile, assuming it is an ellipse. ‘--geopositionangle’ The geometric (ignoring pixel values) angle of the semi-major axis with the first FITS axis in degrees.  File: gnuastro.info, Node: Match, Prev: MakeCatalog, Up: Data analysis 7.4 Match ========= Data can come come from different telescopes, filters, software and even different configurations for a single software. As a result, one of the primary things to do after generating catalogs from each of these sources (for example with *note MakeCatalog::), is to find which sources in one catalog correspond to which in the other(s). In other words, to ‘match’ the two catalogs with each other. Gnuastro’s Match program is in charge of such operations. The nearest objects in the two catalogs, within the given aperture, will be found and given as output. The aperture can be a circle or an ellipse with any orientation. * Menu: * Invoking astmatch:: Inputs, outputs and options of Match  File: gnuastro.info, Node: Invoking astmatch, Prev: Match, Up: Match 7.4.1 Invoking Match -------------------- When given two catalogs, Match finds the rows that are nearest to each other within an input aperture. The executable name is ‘astmatch’ with the following general template $ astmatch [OPTION ...] input-1 input-2 One line examples: ## 1D wavelength match (within 5 angstroms) of the two inputs. ## The wavelengths are in the 5th and 10th columns respectively. $ astmatch --aperture=5e-10 --ccol1=5 --ccol2=10 in1.fits in2.txt ## Match the two catalogs with a circular aperture of width 2. ## (Units same as given positional columns). ## (By default two columns are given for `--ccol1' and `--ccol2', ## The number of values to these determines the dimensions). $ astmatch --aperture=2 input1.txt input2.fits ## Similar to before, but the output is created by merging various ## columns from the two inputs: columns 1, RA, DEC from the first ## input, followed by all columns starting with MAG and the 8th ## column from second input and finally the 10th from first input. $ astmatch --aperture=2 input1.txt input2.fits \ --outcols=a1,aRA,aDEC,b/^MAG/,bBRG,a10 ## Match the two catalogs within an elliptical aperture of 1 and 2 ## arcseconds along RA and Dec respectively. $ astmatch --aperture=1/3600,2/3600 in1.fits in2.txt ## Match the RA and DEC columns of the first input with the RA_D ## and DEC_D columns of the second within a 0.5 arcseconds aperture. $ astmatch --ccol1=RA,DEC --ccol2=RA_D,DEC_D --aperture0.5/3600 \ in1.fits in2.fits Two inputs are necessary for Match to start processing. The inputs can be plain text tables or FITS tables, see *note Tables::. Match follows the same basic behavior of all Gnuastro programs as fully described in *note Common program behavior::. If the first input is a FITS file, the common ‘--hdu’ option (see *note Input output options::) should be used to identify the extension. When the second input is FITS, the extension must be specified with ‘--hdu2’. When ‘--quiet’ is not called, Match will print the number of matches found in standard output (on the command-line). If no match was found, no output file will be created (table or log file). When matches are found, by default, the output file(s) will be the re-arranged input tables such that the rows match each other: both output tables will have the same number of rows which are matched with each other. If ‘--outcols’ is called, the output is a single table with rows chosen from either of the two inputs in any order, see the description of ‘--outcols’. If the ‘--logasoutput’ option is called, the output will be a single table with the contents of the log file, see below. If no output file name is given with the ‘--output’ option, then automatic output *note Automatic output:: will be used to determine the output name(s). Depending on ‘--tableformat’ (see *note Input output options::), the output will then be a (possibly multi-extension) FITS file or (possibly two) plain text file(s). When the output is a FITS file, the default re-arranged inputs will be two extensions of the output FITS file. With ‘--outcols’ and ‘--logasoutput’, the FITS output will be a single table (in one extension). When the ‘--log’ option is called (see *note Operating mode options::), Match will also create a file named ‘astmatch.fits’ (or ‘astmatch.txt’, depending on ‘--tableformat’, see *note Input output options::) in the directory it is run in. This log table will have three columns. The first and second columns show the matching row/record number (counting from 1) of the first and second input catalogs respectively. The third column is the distance between the two matched positions. The units of the distance are the same as the given coordinates (given the possible ellipticity, see description of ‘--aperture’ below). When ‘--logasoutput’ is called, no log file (with a fixed name) will be created. In this case, the output file (possibly given by the ‘--output’ option) will have the contents of this log file. ‘-H STR’ ‘--hdu2=STR’ The extension/HDU of the second input if it is a FITS file. When it isn’t a FITS file, this option’s value is ignored. For the first input, the common option ‘--hdu’ must be used. ‘--outcols=STR’ Columns from both inputs to write into a single matched table output. The value to ‘--outcols’ must be a comma-separated list of strings, for example ‘--outcols=a1,bRA,bDEC’. The first character of each string specifies the input catalog: ‘a’ for the first and ‘b’ for the second. The rest of the characters of the string will be directly used to identify the proper column(s) in the respective table. See *note Selecting table columns:: for how columns can be specified in Gnuastro. In this example, the output will have three columns: the first column of the first input and the ‘RA’ and ‘DEC’ columns of the second input. Another example is given in the one-line examples above. Compared to the default case (where two tables with all their columns) are printed, using this option is much faster: it will only read and re-arrange the necessary columns and it will write a single output table. Combined with regular expressions in large tables, this can be a very powerful and convenient way to retrieve your desired information and do the match at the same time. ‘-l’ ‘--logasoutput’ The output file will have the contents of the log file: indexs in the two catalogs that match with each other along with their distance. See description above. When this option is called, a log file called ‘astmatch.txt’ will not be created. With this option, the default output behavior (two tables containing the re-arranged inputs) will be ‘--notmatched’ Write the non-matching rows into the outputs, not the matched ones. Note that with this option, the two output tables will not necessarily have the same number of rows. Therefore, this option cannot be called with ‘--outcols’. ‘--outcols’ prints mixed columns from both inputs, so they must all have the same number of elements and must correspond to each other. ‘-c INT/STR[,INT/STR]’ ‘--ccol1=INT/STR[,INT/STR]’ The coordinate columns of the first input. The number of dimensions for the match is determined by the number of comma-separated values given to this option. The values can be the column number (counting from 1), exact column name or a regular expression. For more, see *note Selecting table columns::. See the one-line examples above for some usages of this option. ‘-C INT/STR[,INT/STR]’ ‘--ccol2=INT/STR[,INT/STR]’ The coordinate columns of the second input. See the example in ‘--ccol1’ for more. ‘-a FLT[,FLT[,FLT]]’ ‘--aperture=FLT[,FLT[,FLT]]’ Parameters of the aperture for matching. The values given to this option can be fractions, for example when the position columns are in units of degrees, ‘1/3600’ can be used to ask for one arcsecond. The interpretation of the values depends on the requested dimensions (determined from ‘--ccol1’ and ‘--ccol2’) and how many values are given to this option. 1D match The aperture/interval can only take one value: half of the interval around each point (maximum distance from each point). 2D match In a 2D match, the aperture can be a circle, an ellipse aligned in the axes or an ellipse with a rotated major axis. To simply the usage, you can determine the shape based on the number of free parameters for each. 1 number For example ‘--aperture=2’. The aperture will be a circle of the given radius. The value will be in the same units as the columns in ‘--ccol1’ and ‘--ccol2’). 2 numbers For example ‘--aperture=3,4e-10’. The aperture will be an ellipse (if the two numbers are different) with the respective value along each dimension. The numbers are in units of the first and second axis. In the example above, the semi-axis value along the first axis will be 3 (in units of the first coordinate) and along the second axis will be $4\times10^{-10}$ (in units of the second coordinate). Such values can happen if you are comparing catalogs of a spectra for example. If more than one object exists in the aperture, the nearest will be found along the major axis as described in *note Defining an ellipse::. 3 numbers For example ‘--aperture=2,0.6,30’. The aperture will be an ellipse (if the second value is not 1). The first number is the semi-major axis, the second is the axis ratio and the third is the position angle (in degrees). If multiple matches are found within the ellipse, the distance (to find the nearest) is calculated along the major axis in the elliptical space, see *note Defining an ellipse::.  File: gnuastro.info, Node: Modeling and fittings, Next: High-level calculations, Prev: Data analysis, Up: Top 8 Modeling and fitting ********************** In order to fully understand observations after initial analysis on the image, it is very important to compare them with the existing models to be able to further understand both the models and the data. The tools in this chapter create model galaxies and will provide 2D fittings to be able to understand the detections. * Menu: * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image.  File: gnuastro.info, Node: MakeProfiles, Next: MakeNoise, Prev: Modeling and fittings, Up: Modeling and fittings 8.1 MakeProfiles ================ MakeProfiles will create mock astronomical profiles from a catalog, either individually or together in one output image. In data analysis, making a mock image can act like a calibration tool, through which you can test how successfully your detection technique is able to detect a known set of objects. There are commonly two aspects to detecting: the detection of the fainter parts of bright objects (which in the case of galaxies fade into the noise very slowly) or the complete detection of an over-all faint object. Making mock galaxies is the most accurate (and idealistic) way these two aspects of a detection algorithm can be tested. You also need mock profiles in fitting known functional profiles with observations. MakeProfiles was initially built for extra galactic studies, so currently the only astronomical objects it can produce are stars and galaxies. We welcome the simulation of any other astronomical object. The general outline of the steps that MakeProfiles takes are the following: 1. Build the full profile out to its truncation radius in a possibly over-sampled array. 2. Multiply all the elements by a fixed constant so its total magnitude equals the desired total magnitude. 3. If ‘--individual’ is called, save the array for each profile to a FITS file. 4. If ‘--nomerged’ is not called, add the overlapping pixels of all the created profiles to the output image and abort. Using input values, MakeProfiles adds the World Coordinate System (WCS) headers of the FITS standard to all its outputs (except PSF images!). For a simple test on a set of mock galaxies in one image, there is no need for the third step or the WCS information. However in complicated simulations like weak lensing simulations, where each galaxy undergoes various types of individual transformations based on their position, those transformations can be applied to the different individual images with other programs. After all the transformations are applied, using the WCS information in each individual profile image, they can be merged into one output image for convolution and adding noise. * Menu: * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles.  File: gnuastro.info, Node: Modeling basics, Next: If convolving afterwards, Prev: MakeProfiles, Up: MakeProfiles 8.1.1 Modeling basics --------------------- In the subsections below, first a review of some very basic information and concepts behind modeling a real astronomical image is given. You can skip this subsection if you are already sufficiently familiar with these concepts. * Menu: * Defining an ellipse:: An ellipse on a pixelated grid. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model.  File: gnuastro.info, Node: Defining an ellipse, Next: PSF, Prev: Modeling basics, Up: Modeling basics 8.1.1.1 Defining an ellipse ........................... The PSF, see *note PSF::, and galaxy radial profiles are generally defined on an ellipse. Therefore, in this section we’ll start defining an ellipse on a pixelated 2D surface. Labeling the major axis of an ellipse $a$, and its minor axis with $b$, the _axis ratio_ is defined as: $q\equiv b/a$. The major axis of an ellipse can be aligned in any direction, therefore the angle of the major axis with respect to the horizontal axis of the image is defined to be the _position angle_ of the ellipse and in this book, we show it with $\theta$. Our aim is to put a radial profile of any functional form $f(r)$ over an ellipse. Hence we need to associate a radius/distance to every point in space. Let’s define the radial distance $r_{el}$ as the distance on the major axis to the center of an ellipse which is located at $i_c$ and $j_c$ (in other words $r_{el}\equiv{a}$). We want to find $r_{el}$ of a point located at $(i,j)$ (in the image coordinate system) from the center of the ellipse with axis ratio $q$ and position angle $\theta$. First the coordinate system is rotated(1) by $\theta$ to get the new rotated coordinates of that point $(i_r,j_r)$: $$i_r(i,j)=+(i_c-i)\cos\theta+(j_c-j)\sin\theta$$ $$j_r(i,j)=-(i_c-i)\sin\theta+(j_c-j)\cos\theta$$ Recall that an ellipse is defined by $(i_r/a)^2+(j_r/b)^2=1$ and that we defined $r_{el}\equiv{a}$. Hence, multiplying all elements of the the ellipse definition with $r_{el}^2$ we get the elliptical distance at this point point located: $r_{el}=\sqrt{i_r^2+(j_r/q)^2}$. To place the radial profiles explained below over an ellipse, $f(r_{el})$ is calculated based on the functional radial profile desired. MakeProfiles builds the profile starting from the nearest element (pixel in an image) in the dataset to the profile center. The profile value is calculated for that central pixel using monte carlo integration, see *note Sampling from a function::. The next pixel is the next nearest neighbor to the central pixel as defined by $r_{el}$. This process goes on until the profile is fully built upto the trunctation radius. This is done fairly efficiently using a breadth first parsing strategy(2) which is implemented through an ordered linked list. Using this approach, we build the profile by expanding the circumference. Not one more extra pixel has to be checked (the calculation of $r_{el}$ from above is not cheap in CPU terms). Another consequence of this strategy is that extending MakeProfiles to three dimensions becomes very simple: only the neighbors of each pixel have to be changed. Everything else after that (when the pixel index and its radial profile have entered the linked list) is the same, no matter the number of dimensions we are dealing with. ---------- Footnotes ---------- (1) Do not confuse the signs of $sin$ with the rotation matrix defined in *note Warping basics::. In that equation, the point is rotated, here the coordinates are rotated and the point is fixed. (2)  File: gnuastro.info, Node: PSF, Next: Stars, Prev: Defining an ellipse, Up: Modeling basics 8.1.1.2 Point Spread Function ............................. Assume we have a ‘point’ source, or a source that is far smaller than the maximum resolution (a pixel). When we take an image of it, it will ‘spread’ over an area. To quantify that spread, we can define a ‘function’. This is how the point spread function or the PSF of an image is defined. This ‘spread’ can have various causes, for example in ground based astronomy, due to the atmosphere. In practice we can never surpass the ‘spread’ due to the diffraction of the lens aperture. Various other effects can also be quantified through a PSF. For example, the simple fact that we are sampling in a discrete space, namely the pixels, also produces a very small ‘spread’ in the image. Convolution is the mathematical process by which we can apply a ‘spread’ to an image, or in other words blur the image, see *note Convolution process::. The Brightness of an object should remain unchanged after convolution, see *note Flux Brightness and magnitude::. Therefore, it is important that the sum of all the pixels of the PSF be unity. The PSF image also has to have an odd number of pixels on its sides so one pixel can be defined as the center. In MakeProfiles, the PSF can be set by the two methods explained below. Parametric functions A known mathematical function is used to make the PSF. In this case, only the parameters to define the functions are necessary and MakeProfiles will make a PSF based on the given parameters for each function. In both cases, the center of the profile has to be exactly in the middle of the central pixel of the PSF (which is automatically done by MakeProfiles). When talking about the PSF, usually, the full width at half maximum or FWHM is used as a scale of the width of the PSF. ‘Gaussian’ In the older papers, and to a lesser extent even today, some researchers use the 2D Gaussian function to approximate the PSF of ground based images. In its most general form, a Gaussian function can be written as: $$f(r)=a \exp \left( -(x-\mu)^2 \over 2\sigma^2 \right)+d$$ Since the center of the profile is pre-defined, $\mu$ and $d$ are constrained. $a$ can also be found because the function has to be normalized. So the only important parameter for MakeProfiles is the $\sigma$. In the Gaussian function we have this relation between the FWHM and $\sigma$: $$\rm{FWHM}_g=2\sqrt{2\ln{2}}\sigma \approx 2.35482\sigma$$ ‘Moffat’ The Gaussian profile is much sharper than the images taken from stars on photographic plates or CCDs. Therefore in 1969, Moffat proposed this functional form for the image of stars: $$f(r)=a \left[ 1+\left( r\over \alpha \right)^2 \right]^{-\beta}$$ Again, $a$ is constrained by the normalization, therefore two parameters define the shape of the Moffat function: $\alpha$ and $\beta$. The radial parameter is $\alpha$ which is related to the FWHM by $$\rm{FWHM}_m=2\alpha\sqrt{2^{1/\beta}-1}$$ Comparing with the PSF predicted from atmospheric turbulence theory with a Moffat function, Trujillo et al.(1) claim that $\beta$ should be 4.765. They also show how the Moffat PSF contains the Gaussian PSF as a limiting case when $\beta\to\infty$. An input FITS image An input image file can also be specified to be used as a PSF. If the sum of its pixels are not equal to 1, the pixels will be multiplied by a fraction so the sum does become 1. While the Gaussian is only dependent on the FWHM, the Moffat function is also dependent on $\beta$. Comparing these two functions with a fixed FWHM gives the following results: • Within the FWHM, the functions don’t have significant differences. • For a fixed FWHM, as $\beta$ increases, the Moffat function becomes sharper. • The Gaussian function is much sharper than the Moffat functions, even when $\beta$ is large. ---------- Footnotes ---------- (1) Trujillo, I., J. A. L. Aguerri, J. Cepa, and C. M. Gutierrez (2001). “The effects of seeing on Sérsic profiles - II. The Moffat PSFâ€. In: MNRAS 328, pp. 977—985.  File: gnuastro.info, Node: Stars, Next: Galaxies, Prev: PSF, Up: Modeling basics 8.1.1.3 Stars ............. In MakeProfiles, stars are generally considered to be a point source. This is usually the case for extra galactic studies, were nearby stars are also in the field. Since a star is only a point source, we assume that it only fills one pixel prior to convolution. In fact, exactly for this reason, in astronomical images the light profiles of stars are one of the best methods to understand the shape of the PSF and a very large fraction of scientific research is preformed by assuming the shapes of stars to be the PSF of the image.  File: gnuastro.info, Node: Galaxies, Next: Sampling from a function, Prev: Stars, Up: Modeling basics 8.1.1.4 Galaxies ................ Today, most practitioners agree that the flux of galaxies can be modeled with one or a few generalized de Vaucouleur’s (or Sérsic) profiles. $$I(r) = I_e \exp \left ( -b_n \left[ \left( r \over r_e \right)^{1/n} -1 \right] \right )$$ Gérard de Vaucouleurs (1918-1995) was first to show in 1948 that this function best fits the galaxy light profiles, with the only difference that he held $n$ fixed to a value of 4. 20 years later in 1968, J. L. Sérsic showed that $n$ can have a variety of values and does not necessarily need to be 4. This profile depends on the effective radius ($r_e$) which is defined as the radius which contains half of the profile brightness (see *note Profile magnitude::). $I_e$ is the flux at the effective radius. The Sérsic index $n$ is used to define the concentration of the profile within $r_e$ and $b_n$ is a constant dependent on $n$. MacArthur et al.(1) show that for $n>0.35$, $b_n$ can be accurately approximated using this equation: $$b_n=2n - {1\over 3} + {4\over 405n} + {46\over 25515n^2} + {131\over 1148175n^3}-{2194697\over 30690717750n^4}$$ ---------- Footnotes ---------- (1) MacArthur, L. A., S. Courteau, and J. A. Holtzman (2003). “Structure of Disk-dominated Galaxies. I. Bulge/Disk Parameters, Simulations, and Secular Evolutionâ€. In: ApJ 582, pp. 689—722.  File: gnuastro.info, Node: Sampling from a function, Next: Oversampling, Prev: Galaxies, Up: Modeling basics 8.1.1.5 Sampling from a function ................................ A pixel is the ultimate level of accuracy to gather data, we can’t get any more accurate in one image, this is known as sampling in signal processing. However, the mathematical profiles which describe our models have infinite accuracy. Over a large fraction of the area of astrophysically interesting profiles (for example galaxies or PSFs), the variation of the profile over the area of one pixel is not too significant. In such cases, the elliptical radius ($r_{el}$ of the center of the pixel can be assigned as the final value of the pixel, see *note Defining an ellipse::). As you approach their center, some galaxies become very sharp (their value significantly changes over one pixel’s area). This sharpness increases with smaller effective radius and larger Sérsic values. Thus rendering the central value extremely inaccurate. The first method that comes to mind for solving this problem is integration. The functional form of the profile can be integrated over the pixel area in a 2D integration process. However, unfortunately numerical integration techniques also have their limitations and when such sharp profiles are needed they can become extremely inaccurate. The most accurate method of sampling a continuous profile on a discrete space is by choosing a large number of random points within the boundaries of the pixel and taking their average value (or Monte Carlo integration). This is also, generally speaking, what happens in practice with the photons on the pixel. The number of random points can be set with ‘--numrandom’. Unfortunately, repeating this Monte Carlo process would be extremely time and CPU consuming if it is to be applied to every pixel. In order to not loose too much accuracy, in MakeProfiles, the profile is built using both methods explained below. The building of the profile begins from its central pixel and continues (radially) outwards. Monte Carlo integration is first applied (which yields $F_r$), then the central pixel value ($F_c$) is calculated on the same pixel. If the fractional difference ($|F_r-F_c|/F_r$) is lower than a given tolerance level (specified with ‘--tolerance’) MakeProfiles will stop using Monte Carlo integration and only use the central pixel value. The ordering of the pixels in this inside-out construction is based on $r=\sqrt{(i_c-i)^2+(j_c-j)^2}$, not $r_{el}$, see *note Defining an ellipse::. When the axis ratios are large (near one) this is fine. But when they are small and the object is highly elliptical, it might seem more reasonable to follow $r_{el}$ not $r$. The problem is that the gradient is stronger in pixels with smaller $r$ (and larger $r_{el}$) than those with smaller $r_{el}$. In other words, the gradient is strongest along the minor axis. So if the next pixel is chosen based on $r_{el}$, the tolerance level will be reached sooner and lots of pixels with large fractional differences will be missed. Monte Carlo integration uses a random number of points. Thus, every time you run it, by default, you will get a different distribution of points to sample within the pixel. In the case of large profiles, this will result in a slight difference of the pixels which use Monte Carlo integration each time MakeProfiles is run. To have a deterministic result, you have to fix the random number generator properties which is used to build the random distribution. This can be done by setting the ‘GSL_RNG_TYPE’ and ‘GSL_RNG_SEED’ environment variables and calling MakeProfiles with the ‘--envseed’ option. To learn more about the process of generating random numbers, see *note Generating random numbers::. The seed values are fixed for every profile: with ‘--envseed’, all the profiles have the same seed and without it, each will get a different seed using the system clock (which is accurate to within one microsecond). The same seed will be used to generate a random number for all the sub-pixel positions of all the profiles. So in the former, the sub-pixel points checked for all the pixels undergoing Monte carlo integration in all profiles will be identical. In other words, the sub-pixel points in the first (closest to the center) pixel of all the profiles will be identical with each other. All the second pixels studied for all the profiles will also receive an identical (different from the first pixel) set of sub-pixel points and so on. As long as the number of random points used is large enough or the profiles are not identical, this should not cause any systematic bias.  File: gnuastro.info, Node: Oversampling, Prev: Sampling from a function, Up: Modeling basics 8.1.1.6 Oversampling .................... The steps explained in *note Sampling from a function:: do give an accurate representation of a profile prior to convolution. However, in an actual observation, the image is first convolved with or blurred by the atmospheric and instrument PSF in a continuous space and then it is sampled on the discrete pixels of the camera. In order to more accurately simulate this process, the un-convolved image and the PSF are created on a finer pixel grid. In other words, the output image is a certain odd-integer multiple of the desired size, we can call this ‘oversampling’. The user can specify this multiple as a command-line option. The reason this has to be an odd number is that the PSF has to be centered on the center of its image. An image with an even number of pixels on each side does not have a central pixel. The image can then be convolved with the PSF (which should also be oversampled on the same scale). Finally, image can be sub-sampled to get to the initial desired pixel size of the output image. After this, mock noise can be added as explained in the next section. This is because unlike the PSF, the noise occurs in each output pixel, not on a continuous space like all the prior steps.  File: gnuastro.info, Node: If convolving afterwards, Next: Flux Brightness and magnitude, Prev: Modeling basics, Up: MakeProfiles 8.1.2 If convolving afterwards ------------------------------ In case you want to convolve the image later with a given point spread function, make sure to use a larger image size. After convolution, the profiles become larger and a profile that is normally completely outside of the image might fall within it. On one axis, if you want your final (convolved) image to be $m$ pixels and your PSF is $2n+1$ pixels wide, then when calling MakeProfiles, set the axis size to $m+2n$, not $m$. You also have to shift all the pixel positions of the profile centers on the that axis by $n$ pixels to the positive. After convolution, you can crop the outer $n$ pixels with the section crop box specification of Crop: ‘--section=n:*-n,n:*-n’ assuming your PSF is a square, see *note Crop section syntax::. This will also remove all discrete Fourier transform artifacts (blurred sides) from the final image. To facilitate this shift, MakeProfiles has the options ‘--xshift’, ‘--yshift’ and ‘--prepforconv’, see *note Invoking astmkprof::.  File: gnuastro.info, Node: Flux Brightness and magnitude, Next: Profile magnitude, Prev: If convolving afterwards, Up: MakeProfiles 8.1.3 Flux Brightness and magnitude ----------------------------------- Astronomical data pixels are usually in units of counts(1) or electrons or either one divided by seconds. To convert from the counts to electrons, you will need to know the instrument gain. In any case, they can be directly converted to energy or energy/time using the basic hardware (telescope, camera and filter) information. We will continue the discussion assuming the pixels are in units of energy/time. The _brightness_ of an object is defined as its total detected energy per time. This is simply the sum of the pixels that are associated with that detection by our detection tool for example *note NoiseChisel::(2). The _flux_ of an object is in units of energy/time/area and for a detected object, it is defined as its brightness divided by the area used to collect the light from the source or the telescope aperture (for example in $cm^2$)(3). Knowing the flux ($f$) and distance to the object ($r$), we can calculate its _luminosity_: $L=4{\pi}r^2f$. Therefore, flux and luminosity are intrinsic properties of the object, while brightness depends on our detecting tools (hardware and software). Here we will not be discussing luminosity, but brightness. However, since luminosity is the astrophysically interesting quantity, we also defined it here to avoid possible confusion between these two terms because they both have the same units. Images of astronomical objects span over a very large range of brightness. With the Sun (as the brightest object) being roughly $2.5^{60}=10^{24}$ times brighter than the faintest galaxies we can currently detect. Therefore discussing brightness will be very hard, and astronomers have chosen to use a logarithmic scale to talk about the brightness of astronomical objects. But the logarithm can only be usable with a unit-less and always positive value. Fortunately brightness is always positive and to remove the units we divide the brightness of the object ($B$) by a reference brightness ($B_r$). We then define the resulting logarithmic scale as $magnitude$ through the following relation(4) $$m-m_r=-2.5\log_{10} \left( B \over B_r \right)$$ $m$ is defined as the magnitude of the object and $m_r$ is the pre-defined magnitude of the reference brightness. One particularly easy condition is when $B_r=1$. This will allow us to summarize all the hardware specific parameters discussed above into one number as the reference magnitude which is commonly known as the Zero-point(5) magnitude. ---------- Footnotes ---------- (1) Counts are also known as analog to digital units (ADU). (2) If further processing is done, for example the Kron or Petrosian radii are calculated, then the detected area is not sufficient and the total area that was within the respective radius must be used. (3) For a full object that spans over several pixels, the telescope area should be used to find the flux. However, sometimes, only the brightness per pixel is desired. In such cases this book also _loosely_ uses the term flux. This is only approximately accurate however, since while all the pixels have a fixed area, the pixel size can vary with camera on the telescope. (4) The $-2.5$ factor in the definition of magnitudes is a legacy of the our ancient colleagues and in particular Hipparchus of Nicaea (190-120 BC). (5) When $B=Br=1$, the right side of the magnitude definition will be zero. Hence the name, “zero-pointâ€.  File: gnuastro.info, Node: Profile magnitude, Next: Invoking astmkprof, Prev: Flux Brightness and magnitude, Up: MakeProfiles 8.1.4 Profile magnitude ----------------------- To find the profile brightness or its magnitude, (see *note Flux Brightness and magnitude::), it is customary to use the 2D integration of the flux to infinity. However, in MakeProfiles we do not follow this idealistic approach and apply a more realistic method to find the total brightness or magnitude: the sum of all the pixels belonging to a profile within its predefined truncation radius. Note that if the truncation radius is not large enough, this can be significantly different from the total integrated light to infinity. An integration to infinity is not a realistic condition because no galaxy extends indefinitely (important for high Sérsic index profiles), pixelation can also cause a significant difference between the actual total pixel sum value of the profile and that of integration to infinity, especially in small and high Sérsic index profiles. To be safe, you can specify a large enough truncation radius for such compact high Sérsic index profiles. If oversampling is used then the brightness is calculated using the over-sampled image, see *note Oversampling:: which is much more accurate. The profile is first built in an array completely bounding it with a normalization constant of unity (see *note Galaxies::). Taking $B$ to be the desired brightness and $S$ to be the sum of the pixels in the created profile, every pixel is then multiplied by $B/S$ so the sum is exactly $B$. If the ‘--individual’ option is called, this same array is written to a FITS file. If not, only the overlapping pixels of this array and the output image are kept and added to the output array.  File: gnuastro.info, Node: Invoking astmkprof, Prev: Profile magnitude, Up: MakeProfiles 8.1.5 Invoking MakeProfiles --------------------------- MakeProfiles will make any number of profiles specified in a catalog either individually or in one image. The executable name is ‘astmkprof’ with the following general template $ astmkprof [OPTION ...] [Catalog] One line examples: ## Make an image with profiles in catalog.txt (with default size): $ astmkprof catalog.txt ## Make the profiles in catalog.txt over image.fits: $ astmkprof --background=image.fits catalog.txt ## Make a Moffat PSF with FWHM 3pix, beta=2.8, truncation=5 $ astmkprof --kernel=moffat,2.8,5 --oversample=1 ## Make profiles in catalog, using RA and Dec in the given column: $ astmkprof --ccol=RA_CENTER --ccol=DEC_CENTER --mode=wcs catalog.txt ## Make a 1500x1500 merged image (oversampled 500x500) image along ## with an individual image for all the profiles in catalog: $ astmkprof --individual --oversample 3 --naxis=500,500 catalog.txt The parameters of the mock profiles can either be given through a catalog (which stores the parameters of many mock profiles, see *note MakeProfiles catalog::), or the ‘--kernel’ option (see *note MakeProfiles output dataset::). The catalog can be in the FITS ASCII, FITS binary format, or plain text formats (see *note Tables::). The columns related to each parameter can be determined both by number, or by match/search criteria using the column names, units, or comments. with the options ending in ‘col’, see below. Without any file given to the ‘--background’ option, MakeProfiles will make a zero-valued image and build the profiles on that (its size and main WCS parameters can also be defined through the options described in *note MakeProfiles output dataset::). Besides the main/merged image containing all the profiles in the catalog, it is also possible to build individual images for each profile (only enclosing one full profile to its truncation radius) with the ‘--individual’ option. If an image is given to the ‘--background’ option, the pixels of that image are used as the background value for every pixel. The flux value of each profile pixel will be added to the pixel in that background value. In this case, the values to all options relating to the output size and WCS will be ignored if specified (for example ‘--oversample’, ‘--naxis’, and ‘--prepforconv’) on the command-line or in the configuration files. The sections below discuss the options specific to MakeProfiles based on context: the input catalog settings which can have many rows for different profiles are discussed in *note MakeProfiles catalog::, in *note MakeProfiles profile settings::, we discuss how you can set general profile settings (that are the same for all the profiles in the catalog). Finally *note MakeProfiles output dataset:: and *note MakeProfiles log file:: discuss the outputs of MakeProfiles and how you can configure them. Besides these, MakeProfiles also supports all the common Gnuastro program options that are discussed in *note Common options::, so please flip through them is well for a more comfortable usage. Please see *note Sufi simulates a detection:: for a very complete tutorial explaining how one could use MakeProfiles in conjunction with other Gnuastro’s programs to make a complete simulated image of a mock galaxy. * Menu: * MakeProfiles catalog:: Required catalog properties. * MakeProfiles profile settings:: Configuration parameters for all profiles. * MakeProfiles output dataset:: The canvas/dataset to build profiles over. * MakeProfiles log file:: A description of the optional log file.  File: gnuastro.info, Node: MakeProfiles catalog, Next: MakeProfiles profile settings, Prev: Invoking astmkprof, Up: Invoking astmkprof 8.1.5.1 MakeProfiles catalog ............................ The catalog containing information about each profile can be in the FITS ASCII, FITS binary, or plain text formats (see *note Tables::). Its columns can be ordered in any desired manner. You can specify which columns belong to which parameters using the set of options discussed below. For example through the ‘--rcol’ and ‘--tcol’ options, you can specify the column that contains the radial parameter for each profile and its truncation respectively. See *note Selecting table columns:: for a thorough discussion on the values to these options. The value for the profile center in the catalog (the ‘--ccol’ option) can be a floating point number so the profile center can be on any sub-pixel position. Note that pixel positions in the FITS standard start from 1 and an integer is the pixel center. So a 2D image actually starts from the position (0.5, 0.5), which is the bottom-left corner of the first pixel. When a ‘--background’ image with WCS information is provided or you specify the WCS parameters with the respective options, you may also use RA and Dec to identify the center of each profile (see the ‘--mode’ option below). In MakeProfiles, profile centers do not have to be in (overlap with) the final image. Even if only one pixel of the profile within the truncation radius overlaps with the final image size, the profile is built and included in the final image image. Profiles that are completely out of the image will not be created (unless you explicity ask for it with the ‘--individual’ option). You can use the output log file (created with ‘--log’ to see which profiles were within the image, see *note Common options::. If PSF profiles (Moffat or Gaussian, see *note PSF::) are in the catalog and the profiles are to be built in one image (when ‘--individual’ is not used), it is assumed they are the PSF(s) you want to convolve your created image with. So by default, they will not be built in the output image but as separate files. The sum of pixels of these separate files will also be set to unity (1) so you are ready to convolve, see *note Convolution process::. As a summary, the position and magnitude of PSF profile will be ignored. This behavior can be disabled with the ‘--psfinimg’ option. If you want to create all the profiles separately (with ‘--individual’) and you want the sum of the PSF profile pixels to be unity, you have to set their magnitudes in the catalog to the zero-point magnitude and be sure that the central positions of the profiles don’t have any fractional part (the PSF center has to be in the center of the pixel). The list of options directly related to the input catalog columns is shown below. ‘--ccol=STR/INT’ Center coordinate column for each dimension. This option must be called two times to define the center coordinates in an image. For example ‘--ccol=RA’ and ‘--ccol=DEC’ (along with ‘--mode=wcs’) will inform MakeProfiles to look into the catalog columns named ‘RA’ and ‘DEC’ for the Right Ascension and Declination of the profile centers. ‘--fcol=INT/STR’ The functional form of the profile with one of the values below depending on the desired profile. The column can contain either the numeric codes (for example ‘‘1’’) or string characters (for example ‘‘sersic’’). The numeric codes are easier to use in scripts which generate catalogs with hundreds or thousands of profiles. The string format can be easier when the catalog is to be written/checked by hand/eye before running MakeProfiles. It is much more readable and provides a level of documentation. All Gnuastro’s recognized table formats (see *note Recognized table formats::) accept string type columns. To have string columns in a plain text table/catalog, see *note Gnuastro text table format::. • Sérsic profile with ‘‘sersic’’ or ‘‘1’’. • Moffat profile with ‘‘moffat’’ or ‘‘2’’. • Gaussian profile with ‘‘gaussian’’ or ‘‘3’’. • Point source with ‘‘point’’ or ‘‘4’’. • Flat profile with ‘‘flat’’ or ‘‘5’’. • Circumference profile with ‘‘circum’’ or ‘‘6’’. A fixed value will be used for all pixels between the truncation radius ($r_t$) and $r_t-w$ ($w$ is the value to the ‘--circumwidth’). • Radial distance profile with ‘‘distance’’ or ‘‘7’’. At the lowest level, each pixel only has an elliptical radial distance given the profile’s shape and orentiation (see *note Defining an ellipse::). When this profile is chosen, the pixel’s elliptical radial distance from the profile center is written as its value. For this profile, the value in the magnitude column (‘--mcol’) will be ignored. You can use this for checks or as a first approximation to define your own higher-level radial function. In the latter case, just note that the central values are going to be incorrect (see *note Sampling from a function::). ‘--rcol=STR/INT’ The radius parameter of the profiles. Effective radius ($r_e$) if Sérsic, FWHM if Moffat or Gaussian. ‘--ncol=STR/INT’ The Sérsic index ($n$) or Moffat $\beta$. ‘--pcol=STR/INT’ The position angle (in degrees) of the profiles relative to the first FITS axis (horizontal when viewed in SAO ds9). ‘--qcol=STR/INT’ The axis ratio of the profiles (minor axis divided by the major axis in a 2D ellipse). ‘--mcol=STR/INT’ The total pixelated magnitude of the profile within the truncation radius, see *note Profile magnitude::. ‘--tcol=STR/INT’ The truncation radius of this profile. By default it is in units of the radial parameter of the profile (the value in the ‘--rcol’ of the catalog). If ‘--tunitinp’ is given, this value is interpreted in units of pixels (prior to oversampling) irrespective of the profile.  File: gnuastro.info, Node: MakeProfiles profile settings, Next: MakeProfiles output dataset, Prev: MakeProfiles catalog, Up: Invoking astmkprof 8.1.5.2 MakeProfiles profile settings ..................................... The profile parameters that differ between each created profile are specified through the columns in the input catalog and described in *note MakeProfiles catalog::. Besides those there are general settings for some profiles that don’t differ between one profile and another, they are a property of the general process. For example how many random points to use in the monte-carlo integration, this value is fixed for all the profiles. The options described in this section are for configuring such properties. ‘--mode=STR’ Interpret the center position columns (‘--ccol’ in *note MakeProfiles catalog::) in image or WCS coordinates. This option thus accepts only two values: ‘img’ and ‘wcs’. It is mandatory when a catalog is being used as input. ‘-r’ ‘--numrandom’ The number of random points used in the central regions of the profile, see *note Sampling from a function::. ‘-e’ ‘--envseed’ Use the value to the ‘GSL_RNG_SEED’ environment variable to generate the random Monte Carlo sampling distribution, see *note Sampling from a function:: and *note Generating random numbers::. ‘-t FLT’ ‘--tolerance=FLT’ The tolerance to switch from Monte Carlo integration to the central pixel value, see *note Sampling from a function::. ‘-p’ ‘--tunitinp’ The truncation column of the catalog is in units of pixels. By default, the truncation column is considered to be in units of the radial parameters of the profile (‘--rcol’). Read it as ‘t-unit-in-p’ for ‘truncation unit in pixels’. ‘-f’ ‘--mforflatpix’ When making fixed value profiles (flat and circumference, see ‘‘--fcol’’), don’t use the value in the column specified by ‘‘--mcol’’ as the magnitude. Instead use it as the exact value that all the pixels of these profiles should have. This option is irrelevant for other types of profiles. This option is very useful for creating masks, or labeled regions in an image. Any integer, or floating point value can used in this column with this option, including ‘NaN’ (or ‘‘nan’’, or ‘‘NAN’’, case is irrelevant), and infinities (‘inf’, ‘-inf’, or ‘+inf’). For example, with this option if you set the value in the magnitude column (‘--mcol’) to ‘NaN’, you can create an elliptical or circular mask over an image (which can be given as the argument), see *note Blank pixels::. Another useful application of this option is to create labeled elliptical or circular apertures in an image. To do this, set the value in the magnitude column to the label you want for this profile. This labeled image can then be used in combination with NoiseChisel’s output (see *note NoiseChisel output::) to do aperture photometry with MakeCatalog (see *note MakeCatalog::). Alternatively, if you want to mark regions of the image (for example with an elliptical circumference) and you don’t want to use NaN values (as explained above) for some technical reason, you can get the minimum or maximum value in the image (1) using Arithmetic (see *note Arithmetic::), then use that value in the magnitude column along with this option for all the profiles. Please note that when using MakeProfiles on an already existing image, you have to set ‘‘--oversample=1’’. Otherwise all the profiles will be scaled up based on the oversampling scale in your configuration files (see *note Configuration files::) unless you have accounted for oversampling in your catalog. ‘--mcolisbrightness’ The value given in the “magnitude column†(specified by ‘--mcol’, see *note MakeProfiles catalog::) must be interpretted as brightness, not magnitude. The zeropoint magnitude (value to the ‘--zeropoint’ option) is ignored and the given value must have the same units as the input dataset’s pixels. Recall that the total profile magnitude or brightness that is specified with in the ‘--mcol’ column of the input catalog is not an integration to infinity, but the actual sum of pixels in the profile (until the desired truncation radius). See *note Profile magnitude:: for more on this point. ‘--magatpeak’ The magnitude column in the catalog (see *note MakeProfiles catalog::) will be used to find the brightness only for the peak profile pixel, not the full profile. Note that this is the flux of the profile’s peak pixel in the final output of MakeProfiles. So beware of the oversampling, see *note Oversampling::. This option can be useful if you want to check a mock profile’s total magnitude at various truncation radii. Without this option, no matter what the truncation radius is, the total magnitude will be the same as that given in the catalog. But with this option, the total magnitude will become brighter as you increase the truncation radius. In sharper profiles, sometimes the accuracy of measuring the peak profile flux is more than the overall object brightness. In such cases, with this option, the final profile will be built such that its peak has the given magnitude, not the total profile. *CAUTION:* If you want to use this option for comparing with observations, please note that MakeProfiles does not do convolution. Unless you have de-convolved your data, your images are convolved with the instrument and atmospheric PSF, see *note PSF::. Particularly in sharper profiles, the flux in the peak pixel is strongly decreased after convolution. Also note that in such cases, besides de-convolution, you will have to set ‘--oversample=1’ otherwise after resampling your profile with Warp (see *note Warp::), the peak flux will be different. ‘-X INT,INT’ ‘--shift=INT,INT’ Shift all the profiles and enlarge the image along each dimension. To better understand this option, please see $n$ in *note If convolving afterwards::. This is useful when you want to convolve the image afterwards. If you are using an external PSF, be sure to oversample it to the same scale used for creating the mock images. If a background image is specified, any possible value to this option is ignored. ‘-c’ ‘--prepforconv’ Shift all the profiles and enlarge the image based on half the width of the first Moffat or Gaussian profile in the catalog, considering any possible oversampling see *note If convolving afterwards::. ‘--prepforconv’ is only checked and possibly activated if ‘--xshift’ and ‘--yshift’ are both zero (after reading the command-line and configuration files). If a background image is specified, any possible value to this option is ignored. ‘-z FLT’ ‘--zeropoint=FLT’ The zero-point magnitude of the image. ‘-w FLT’ ‘--circumwidth=FLT’ The width of the circumference if the profile is to be an elliptical circumference or annulus. See the explanations for this type of profile in ‘--fcol’. ‘-R’ ‘--replace’ Do not add the pixels of each profile over the background (possibly crowded by other profiles), replace them. By default, when two profiles overlap, the final pixel value is the sum of all the profiles that overlap on that pixel. When this option is given, the pixels are not added but replaced by the newer profile’s pixel and any value under it is lost. When order matters, make sure to use this function with ‘‘--numthreads=1’’. When multiple threads are used, the separate profiles are built asynchronously and not in order. Since order does not matter in an addition, this causes no problems by default but has to be considered when this option is given. Using multiple threads is no problem if the profiles are to be used as a mask with a blank or fixed value (see ‘‘--mforflatpix’’) since all their pixel values are the same. Note that only non-zero pixels are replaced. With radial profiles (for example Sérsic or Moffat) only values above zero will be part of the profile. However, when using flat profiles with the ‘‘--mforflatpix’’ option, you should be careful not to give a ‘0.0’ value as the flat profile’s pixel value. ---------- Footnotes ---------- (1) The minimum will give a better result, because the maximum can be too high compared to most pixels in the image, making it harder to display.  File: gnuastro.info, Node: MakeProfiles output dataset, Next: MakeProfiles log file, Prev: MakeProfiles profile settings, Up: Invoking astmkprof 8.1.5.3 MakeProfiles output dataset ................................... MakeProfiles takes an input catalog uses basic properties that are defined there to build a dataset, for example a 2D image containing the profiles in the catalog. In *note MakeProfiles catalog:: and *note MakeProfiles profile settings::, the catalog and profile settings were discussed. The options of this section, allow you to configure the output dataset (or the canvas that will host the built profiles). ‘-k STR’ ‘--background=STR’ A background image FITS file to build the profiles on. The extension that contains the image should be specified with the ‘--backhdu’ option, see below. When a background image is specified, it will be used to derive all the information about the output image. Hence, the following options will be ignored: ‘--naxis’, ‘--oversample’, ‘--crpix’, ‘--crval’ (generally, all other WCS related parameters) and the output’s data type (see ‘--type’ in *note Input output options::). The image will act like a canvas to build the profiles on: profile pixel values will be summed with the background image pixel values. With the ‘--replace’ option you can disable this behavior and replace the profile pixels with the background pixels. If you want to use all the image information above, except for the pixel values (you want to have a blank canvas to build the profiles on, based on an input image), you can call ‘--clearcanvas’, to set all the input image’s pixels to zero before starting to build the profiles over it (this is done in memory after reading the input, so nothing will happen to your input file). ‘-B STR/INT’ ‘--backhdu=STR/INT’ The header data unit (HDU) of the file given to ‘--background’. ‘-C’ ‘--clearcanvas’ When an input image is specified (with the ‘--background’ option, set all its pixels to 0.0 immediately after reading it into memory. Effectively, this will allow you to use all its properties (described under the ‘--background’ option), without having to worry about the pixel values. ‘--clearcanvas’ can come in handy in many situations, for example if you want to create a labeled image (segmentation map) for creating a catalog (see *note MakeCatalog::). In other cases, you might have modeled the objects in an image and want to create them on the same frame, but without the original pixel values. ‘-E STR/INT,FLT[,FLT,[...]]’ ‘--kernel=STR/INT,FLT[,FLT,[...]]’ Only build one kernel profile with the parameters given as the values to this option. The different values must be separated by a comma (<,>). The first value identifies the radial function of the profile, either through a string or through a number (see description of ‘--fcol’ in *note MakeProfiles catalog::). Each radial profile needs a different total number of parameters: Sérsic and Moffat functions need 3 parameters: radial, Sérsic index or Moffat $\beta$, and truncation radius. The Gaussian function needs two parameters: radial and truncation radius. The point function doesn’t need any parameters and flat and circumference profiles just need one parameter (truncation radius). The PSF or kernel is a unique (and highly constrained) type of profile: the sum of its pixels must be one, its center must be the center of the central pixel (in an image with an odd number of pixels on each side), and commonly it is circular, so its axis ratio and position angle are one and zero respectively. Kernels are commonly necessary for various data analysis and data manipulation steps (for example see *note Convolve::, and *note NoiseChisel::. Because of this it is inconvenient to define a catalog with one row and many zero valued columns (for all the non-necessary parameters). Hence, with this option, it is possible to create a kernel with MakeProfiles without the need to create a catalog. Here are some examples: ‘--kernel=moffat,3,2.8,5’ A Moffat kernel with FWHM of 3 pixels, $\beta=2.8$ which is truncated at 5 times the FWHM. ‘--kernel=gaussian,2,3’ A Gaussian kernel with FWHM of 2 pixels and truncated at 3 times the FWHM. ‘-x INT,INT’ ‘--naxis=INT,INT’ The number of pixels along each dimension axis of the output in FITS order. This is before over-sampling. For example if you call MakeProfiles with ‘--naxis=100,150 --oversample=5’ (assuming no shift due for later convolution), then the final image size along the first axis will be 500 by 750 pixels. Fractions are acceptable as values for each dimension, however, they must reduce to an integer, so ‘--naxis=150/3,300/3’ is acceptable but ‘--naxis=150/4,300/4’ is not. When viewing a FITS image in DS9, the first FITS dimension is in the horizontal direction and the second is vertical. As an example, the image created with the example above will have 500 pixels horizontally and 750 pixels vertically. If a background image is specified, this option is ignored. ‘-s INT’ ‘--oversample=INT’ The scale to over-sample the profiles and final image. If not an odd number, will be added by one, see *note Oversampling::. Note that this ‘--oversample’ will remain active even if an input image is specified. If your input catalog is based on the background image, be sure to set ‘--oversample=1’. ‘--psfinimg’ Build the possibly existing PSF profiles (Moffat or Gaussian) in the catalog into the final image. By default they are built separately so you can convolve your images with them, thus their magnitude and positions are ignored. With this option, they will be built in the final image like every other galaxy profile. To have a final PSF in your image, make a point profile where you want the PSF and after convolution it will be the PSF. ‘-i’ ‘--individual’ If this option is called, each profile is created in a separate FITS file within the same directory as the output and the row number of the profile (starting from zero) in the name. The file for each row’s profile will be in the same directory as the final combined image of all the profiles and will have the final image’s name as a suffix. So for example if the final combined image is named ‘./out/fromcatalog.fits’, then the first profile that will be created with this option will be named ‘./out/0_fromcatalog.fits’. Since each image only has one full profile out to the truncation radius the profile is centered and so, only the sub-pixel position of the profile center is important for the outputs of this option. The output will have an odd number of pixels. If there is no oversampling, the central pixel will contain the profile center. If the value to ‘--oversample’ is larger than unity, then the profile center is on any of the central ‘--oversample’’d pixels depending on the fractional value of the profile center. If the fractional value is larger than half, it is on the bottom half of the central region. This is due to the FITS definition of a real number position: The center of a pixel has fractional value $0.00$ so each pixel contains these fractions: .5 – .75 – .00 (pixel center) – .25 – .5. ‘-m’ ‘--nomerged’ Don’t make a merged image. By default after making the profiles, they are added to a final image with side lengths specified by ‘--naxis’if they overlap with it. The options below can be used to define the world coordinate system (WCS) properties of the MakeProfiles outputs. The option names are delibarately chosen to be the same as the FITS standard WCS keywords. See Section 8 of Pence et al [2010] (https://doi.org/10.1051/0004-6361/201015362) for a short introduction to WCS in the FITS standard(1). If you look into the headers of a FITS image with WCS for example you will see all these names but in uppercase and with numbers to represent the dimensions, for example ‘CRPIX1’ and ‘PC2_1’. You can see the FITS headers with Gnuastro’s *note Fits:: program using a command like this: ‘$ astfits -p image.fits’. If the values given to any of these options does not correspond to the number of dimensions in the output dataset, then no WCS information will be added. ‘--crpix=FLT,FLT’ The pixel coordinates of the WCS reference point. Fractions are acceptable for the values of this option. ‘--crval=FLT,FLT’ The WCS coordinates of the Reference point. Fractions are acceptable for the values of this option. ‘--cdelt=FLT,FLT’ The resolution (size of one data-unit or pixel in WCS units) of the non-oversampled dataset. Fractions are acceptable for the values of this option. ‘--pc=FLT,FLT,FLT,FLT’ The PC matrix of the WCS rotation, see the FITS standard (link above) to better understand the PC matrix. ‘--cunit=STR,STR’ The units of each WCS axis, for example ‘deg’. Note that these values are part of the FITS standard (link above). MakeProfiles won’t complain if you use non-standard values, but later usage of them might cause trouble. ‘--ctype=STR,STR’ The type of each WCS axis, for example ‘RA---TAN’ and ‘DEC--TAN’. Note that these values are part of the FITS standard (link above). MakeProfiles won’t complain if you use non-standard values, but later usage of them might cause trouble. ---------- Footnotes ---------- (1) The world coordinate standard in FITS is a very beatiful and powerful concept to link/associate datasets with the outside world (other datasets). The description in the FITS standard (link above) only touches the tip of the ice-burg. To learn more please see Greisen and Calabretta [2002] (https://doi.org/10.1051/0004-6361:20021326), Calabretta and Greisen [2002] (https://doi.org/10.1051/0004-6361:20021327), Greisen et al. [2006] (https://doi.org/10.1051/0004-6361:20053818), and Calabretta et al. (http://www.atnf.csiro.au/people/mcalabre/WCS/dcs_20040422.pdf)  File: gnuastro.info, Node: MakeProfiles log file, Prev: MakeProfiles output dataset, Up: Invoking astmkprof 8.1.5.4 MakeProfiles log file ............................. Besides the final merged dataset of all the profiles, or the individual datasets (see *note MakeProfiles output dataset::), if the ‘--log’ option is called MakeProfiles will also create a log file in the current directory (where you run MockProfiles). See *note Common options:: for a full description of ‘--log’ and other options that are shared between all Gnuastro programs. The values for each column are explained in the first few commented lines of the log file (starting with ‘#’ character). Here is a more complete description. • An ID (row number of profile in input catalog). • The total magnitude of the profile in the output dataset. When the profile does not completely overlap with the output dataset, this will be different from your input magnitude. • The number of pixels (in the oversampled image) which used Monte Carlo integration and not the central pixel value, see *note Sampling from a function::. • The fraction of flux in the Monte Carlo integrated pixels. • If an individual image was created, this column will have a value of ‘1’, otherwise it will have a value of ‘0’.  File: gnuastro.info, Node: MakeNoise, Prev: MakeProfiles, Up: Modeling and fittings 8.2 MakeNoise ============= Real data are always buried in noise, therefore to finalize a simulation of real data (for example to test our observational algorithms) it is essential to add noise to the mock profiles created with MakeProfiles, see *note MakeProfiles::. Below, the general principles and concepts to help understand how noise is quantified is discussed. MakeNoise options and argument are then discussed in *note Invoking astmknoise::. * Menu: * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise.  File: gnuastro.info, Node: Noise basics, Next: Invoking astmknoise, Prev: MakeNoise, Up: MakeNoise 8.2.1 Noise basics ------------------ Deep astronomical images, like those used in extragalactic studies seriously suffer from noise in the data. Generally speaking, the sources of noise in an astronomical image are photon counting noise and Instrumental noise which are discussed in detail below. We finish with a short introduction on how random numbers are generated and how you can determine the random number generator and seed value. * Menu: * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated.  File: gnuastro.info, Node: Photon counting noise, Next: Instrumental noise, Prev: Noise basics, Up: Noise basics 8.2.1.1 Photon counting noise ............................. Thanks to the very accurate electronics used in today’s detectors, this type of noise is the main cause of concern for extra galactic studies. It can generally be associate with the counting error that is known to have a Poisson distribution. The Poisson distribution is about counting. But counting is a discrete operation with only positive values, for example we can’t count $3.2$ or $-2$ of anything. We only count $0$, $1$, $2$, $3$ and so on. Therefore the Poisson distribution is also a discrete distribution, only applying to whole positive integers. Let’s assume the mean value of counting something is known. In this case, we are counting the number of electrons that are produced by photons in a detector (for example CCD) pixel. Let’s call this mean $\lambda$. Furthermore, let’s take $k$ to represent the result of one particular counting attempt. The probability density function of $k$ can be written as: $$f(k)={\lambda^k \over k!} e^{-\lambda},\quad k\in {0, 1, 2, 3, \dots }$$ Because the Poisson distribution is only applicable to positive values, naturally it is very skewed when $\lambda$ is near zero. One qualitative way to explain it is that there simply aren’t enough integers smaller than $\lambda$, than integers that are larger than it. Therefore to accommodate all possibilities, it has to be skewed when $\lambda$ is small. But as $\lambda$ becomes larger and larger, the distribution becomes more and more symmetric. One very useful property of the Poisson distribution is that the mean value is also its variance. When $\lambda$ is very large, say $\lambda>1000$, then the normal (Gaussian) distribution, see *note PSF::, is an excellent approximation of the Poisson distribution with mean $\mu=\lambda$ and standard deviation $\sigma=\sqrt{\lambda}$. We see that the variance or dispersion of the distribution depends on the mean value, and when it is large it can be approximated with a Gaussian that only has one free parameter ($\mu=\lambda$ and $\sigma=\sqrt{\lambda}$) instead of two that it originally has. The astronomical objects after convolution with the PSF of the instrument, lie above a certain background flux. This background flux is defined to be the average flux of a region in the image that has absolutely no objects. The physical origin of this background value is the brightness of the atmosphere or possible stray light within the imaging instrument. It is thus an ideal definition, because in practice, what lies deep in the noise far lower than the detection limit is never known(1). However, in a real image, a relatively large number of very faint objects can been fully buried in the noise. These undetected objects will bias the background measurement to slightly larger values. The sky value is therefore defined to be the average of the undetected regions in the image, so in an ideal case where all the objects have been detected, the sky value and background value are the same. As longer wavelengths are used, the background value becomes more significant and also varies over a wide image field. Such variations are not currently implemented in MakeProfiles, but will be in the future. In a mock image, we have the luxury of setting the background value. In each pixel of the canvas of pixels, the flux is the sum of contributions from various sources after convolution. Let’s name this flux of the convolved sum of possibly overlapping objects, $I_{nn}$. $nn$ representing ‘no noise’. For now, let’s assume the background is constant and represented by $B$. In practice the background values are larger than $\sim1,000$ counts. Then the flux after adding noise is a random value taken from a Gaussian distribution with the following mean ($\mu$) and standard deviation ($\sigma$): $$\mu=B+I_{nn}, \quad \sigma=\sqrt{B+I_{nn}}$$ Since this type of noise is inherent in the objects we study, it is usually measured on the same scale as the astronomical objects, namely the magnitude system, see *note Flux Brightness and magnitude::. It is then internally converted to the flux scale for further processing. ---------- Footnotes ---------- (1) See the section on sky in Akhlaghi M., Ichikawa. T. 2015. Astrophysical Journal Supplement Series.  File: gnuastro.info, Node: Instrumental noise, Next: Final noised pixel value, Prev: Photon counting noise, Up: Noise basics 8.2.1.2 Instrumental noise .......................... While taking images with a camera, a dark current is fed to the pixels, the variation of the value of this dark current over the pixels, also adds to the final image noise. Another source of noise is the readout noise that is produced by the electronics in the CCD that attempt to digitize the voltage produced by the photo-electrons in the analog to digital converter. In deep extra-galactic studies these sources of noise are not as significant as the noise of the background sky. Let $C$ represent the combined standard deviation of all these sources of noise. If only this source of noise is present, the noised pixel value would be a random value chosen from a Gaussian distribution with $$\mu=I_{nn}, \quad \sigma=\sqrt{C^2+I_{nn}}$$ This type of noise is completely independent of the type of objects being studied, it is completely determined by the instrument. So the flux scale (and not magnitude scale) is most commonly used for this type of noise. In practice, this value is usually reported in ADUs not flux or electron counts. The gain value of the device can be used to convert between these two, see *note Flux Brightness and magnitude::.  File: gnuastro.info, Node: Final noised pixel value, Next: Generating random numbers, Prev: Instrumental noise, Up: Noise basics 8.2.1.3 Final noised pixel value ................................ Depending on the values you specify for $B$ and $C$ from the above, the final noised value for each pixel is a random value chosen from a Gaussian distribution with $$\mu=B+I_{nn}, \quad \sigma=\sqrt{C^2+B+I_{nn}}$$  File: gnuastro.info, Node: Generating random numbers, Prev: Final noised pixel value, Up: Noise basics 8.2.1.4 Generating random numbers ................................. As discussed above, to generate noise we need to make random samples of a particular distribution. So it is important to understand some general concepts regarding the generation of random numbers. For a very complete and nice introduction we strongly advise reading Donald Knuth’s “The art of computer programmingâ€, volume 2, chapter 3(1). Quoting from the GNU Scientific Library manual, “If you don’t own it, you should stop reading right now, run to the nearest bookstore, and buy itâ€(2)! Using only software, we can only produce what is called a psudo-random sequence of numbers. A true random number generator is a hardware (let’s assume we have made sure it has no systematic biases), for example throwing dice or flipping coins (which have remained from the ancient times). More modern hardware methods use atmospheric noise, thermal noise or other types of external electromagnetic or quantum phenomena. All psudo-random number generators (software) require a seed to be the basis of the generation. The advantage of having a seed is that if you specify the same seed for multiple runs, you will get an identical sequence of random numbers which allows you to reproduce the same final noised image. The programs in GNU Astronomy Utilities (for example MakeNoise or MakeProfiles) use the GNU Scientific Library (GSL) to generate random numbers. GSL allows the user to set the random number generator through environment variables, see *note Installation directory:: for an introduction to environment variables. In the chapter titled “Random Number Generation†they have fully explained the various random number generators that are available (there are a lot of them!). Through the two environment variables ‘GSL_RNG_TYPE’ and ‘GSL_RNG_SEED’ you can specify the generator and its seed respectively. If you don’t specify a value for ‘GSL_RNG_TYPE’, GSL will use its default random number generator type. The default type is sufficient for most general applications. If no value is given for the ‘GSL_RNG_SEED’ environment variable and you have asked Gnuastro to read the seed from the environment (through the ‘--envseed’ option), then GSL will use the default value of each generator to give identical outputs. If you don’t explicitly tell Gnuastro programs to read the seed value from the environment variable, then they will use the system time (accurate to within a microsecond) to generate (apparently random) seeds. In this manner, every time you run the program, you will get a different random number distribution. There are two ways you can specify values for these environment variables. You can call them on the same command-line for example: $ GSL_RNG_TYPE="taus" GSL_RNG_SEED=345 astmknoise input.fits In this manner the values will only be used for this particular execution of MakeNoise. Alternatively, you can define them for the full period of your terminal session or script length, using the shell’s ‘export’ command with the two separate commands below (for a script remove the ‘$’ signs): $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 The subsequent programs which use GSL’s random number generators will hence forth use these values in this session of the terminal you are running or while executing this script. In case you want to set fixed values for these parameters every time you use the GSL random number generator, you can add these two lines to your ‘.bashrc’ startup script(3), see *note Installation directory::. *NOTE:* If the two environment variables ‘GSL_RNG_TYPE’ and ‘GSL_RNG_SEED’ are defined, GSL will report them by default, even if you don’t use the ‘--envseed’ option. For example you can see the top few lines of the output of MakeProfiles: $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 $ astmkprof catalog.txt --envseed GSL_RNG_TYPE=taus GSL_RNG_SEED=345 MakeProfiles started on AAA BBB DD EE:FF:GG HHH - 6 profiles read from catalog.txt 0.000236 seconds - Random number generator (RNG) type: taus - RNG seed for all profiles: 345 The first two output lines (showing the names of the environment variables) are printed by GSL before MakeProfiles actually starts generating random numbers. The Gnuastro programs will report the values they use independently, you should check them for the final values used. For example if ‘--envseed’ is not given, ‘GSL_RNG_SEED’ will not be used and the last line shown above will not be printed. In the case of MakeProfiles, each profile will get its own seed value. ---------- Footnotes ---------- (1) Knuth, Donald. 1998. The art of computer programming. Addison–Wesley. ISBN 0-201-89684-2 (2) For students, running to the library might be more affordable! (3) Don’t forget that if you are going to give your scripts (that use the GSL random number generator) to others you have to make sure you also tell them to set these environment variable separately. So for scripts, it is best to keep all such variable definitions within the script, even if they are within your ‘.bashrc’.  File: gnuastro.info, Node: Invoking astmknoise, Prev: Noise basics, Up: MakeNoise 8.2.2 Invoking MakeNoise ------------------------ MakeNoise will add noise to an existing image. The executable name is ‘astmknoise’ with the following general template $ astmknoise [OPTION ...] InputImage.fits One line examples: ## Add noise with a standard deviation of 100 to image: $ astmknoise --sigma=100 image.fits ## Add noise to input image assuming a background magnitude (with ## zeropoint magnitude of 0) and a certain instrumental noise: $ astmknoise --background=-10 -z0 --instrumental=20 mockimage.fits If actual processing is to be done, the input image is a mandatory argument. The full list of options common to all the programs in Gnuastro can be seen in *note Common options::. The type (see *note Numeric data types::) of the output can be specified with the ‘--type’ option, see *note Input output options::. The header of the output FITS file keeps all the parameters that were influential in making it. This is done for future reproducibility. ‘-s FLT’ ‘--sigma=FLT’ The total noise sigma in the same units as the pixel values. With this option, the ‘--background’, ‘--zeropoint’ and ‘--instrumental’ will be ignored. With this option, the noise will be independent of the pixel values (which is not realistic, see *note Photon counting noise::). Hence it is only useful if you are working on low surface brightness regions where the change in pixel value (and thus real noise) is insignificant. ‘-b FLT’ ‘--background=FLT’ The background pixel value for the image in units of magnitudes, see *note Photon counting noise:: and *note Flux Brightness and magnitude::. ‘-z FLT’ ‘--zeropoint=FLT’ The zeropoint magnitude used to convert the value of ‘--background’ (in units of magnitude) to flux, see *note Flux Brightness and magnitude::. ‘-i FLT’ ‘--instrumental=FLT’ The instrumental noise which is in units of flux, see *note Instrumental noise::. ‘-e’ ‘--envseed’ Use the ‘GSL_RNG_SEED’ environment variable for the seed used in the random number generator, see *note Generating random numbers::. With this option, the output image noise is always going to be identical (or reproducible). ‘-d’ ‘--doubletype’ Save the output in the double precision floating point format that was used internally. This option will be most useful if the input images were of integer types.  File: gnuastro.info, Node: High-level calculations, Next: Library, Prev: Modeling and fittings, Up: Top 9 High-level calculations ************************* After the reduction of raw data (for example with the programs in *note Data manipulation::) you will have reduced images/data ready for processing/analyzing (for example with the programs in *note Data analysis::). But the processed/analyzed data (or catalogs) are still not enough to derive any scientific result. Even higher-level analysis is still needed to convert the observed magnitudes, sizes or volumes into physical quantities that we associate with each catalog entry or detected object which is the purpose of the tools in this section. * Menu: * CosmicCalculator:: Calculate cosmological variables  File: gnuastro.info, Node: CosmicCalculator, Prev: High-level calculations, Up: High-level calculations 9.1 CosmicCalculator ==================== To derive higher-level information regarding our sources in extra-galactic astronomy, cosmological calculations are necessary. In Gnuastro, CosmicCalculator is in charge of such calculations. Before discussing how CosmicCalculator is called and operates (in *note Invoking astcosmiccal::), it is important to provide a rough but mostly self sufficient review of the basics and the equations used in the analysis. In *note Distance on a 2D curved space:: the basic idea of understanding distances in a curved and expanding 2D universe (which we can visualize) are reviewed. Having solidified the concepts there, in *note Extending distance concepts to 3D::, the formalism is extended to the 3D universe we are trying to study in our research. The focus here is obtaining a physical insight into these equations (mainly for the use in real observational studies). There are many books thoroughly deriving and proving all the equations with all possible initial conditions and assumptions for any abstract universe, interested readers can study those books. * Menu: * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator  File: gnuastro.info, Node: Distance on a 2D curved space, Next: Extending distance concepts to 3D, Prev: CosmicCalculator, Up: CosmicCalculator 9.1.1 Distance on a 2D curved space ----------------------------------- The observations to date (for example the Planck 2015 results), have not measured(1) the presence of significant curvature in the universe. However to be generic (and allow its measurement if it does in fact exist), it is very important to create a framework that allows non-zero uniform curvature. However, this section is not intended to be a fully thorough and mathematically complete derivation of these concepts. There are many references available for such reviews that go deep into the abstract mathematical proofs. The emphasis here is on visualization of the concepts for a beginner. As 3D beings, it is difficult for us to mentally create (visualize) a picture of the curvature of a 3D volume. Hence, here we will assume a 2D surface/space and discuss distances on that 2D surface when it is flat and when it is curved. Once the concepts have been created/visualized here, we will extend them, in *note Extending distance concepts to 3D::, to a real 3D spatial _slice_ of the Universe we live in and hope to study. To be more understandable (actively discuss from an observer’s point of view) let’s assume there’s an imaginary 2D creature living on the 2D space (which _might_ be curved in 3D). Here, we will be working with this creature in its efforts to analyze distances in its 2D universe. The start of the analysis might seem too mundane, but since it is difficult to imagine a 3D curved space, it is important to review all the very basic concepts thoroughly for an easy transition to a universe that is more difficult to visualize (a curved 3D space embedded in 4D). To start, let’s assume a static (not expanding or shrinking), flat 2D surface similar to *note Figure 9.1: flatplane. and that the 2D creature is observing its universe from point $A$. One of the most basic ways to parametrize this space is through the Cartesian coordinates ($x$, $y$). In *note Figure 9.1: flatplane, the basic axes of these two coordinates are plotted. An infinitesimal change in the direction of each axis is written as $dx$ and $dy$. For each point, the infinitesimal changes are parallel with the respective axes and are not shown for clarity. Another very useful way of parameterizing this space is through polar coordinates. For each point, we define a radius ($r$) and angle ($\phi$) from a fixed (but arbitrary) reference axis. In *note Figure 9.1: flatplane. the infinitesimal changes for each polar coordinate are plotted for a random point and a dashed circle is shown for all points with the same radius. [image src="gnuastro-figures/flatplane.png" text="../gnuastro-figures//flatplane.eps"] Figure 9.1: Two dimensional Cartesian and polar coordinates on a flat plane. Assuming an object is placed at a certain position, which can be parameterized as $(x,y)$, or $(r,\phi)$, a general infinitesimal change in its position will place it in the coordinates $(x+dx,y+dy)$ and $(r+dr,\phi+d\phi)$. The distance (on the flat 2D surface) that is covered by this infinitesimal change in the static universe ($ds_s$, the subscript signifies the static nature of this universe) can be written as: $$ds_s=dx^2+dy^2=dr^2+r^2d\phi^2$$ The main question is this: how can the 2D creature incorporate the (possible) curvature in its universe when it’s calculating distances? The universe that it lives in might equally be a curved surface like *note Figure 9.2: sphereandplane. The answer to this question but for a 3D being (us) is the whole purpose to this discussion. Here, we want to give the 2D creature (and later, ourselves) the tools to measure distances if the space (that hosts the objects) is curved. *note Figure 9.2: sphereandplane. assumes a spherical shell with radius $R$ as the curved 2D plane for simplicity. The 2D plane is tangent to the spherical shell and only touches it at $A$. This idea will be generalized later. The first step in measuring the distance in a curved space is to imagine a third dimension along the $z$ axis as shown in *note Figure 9.2: sphereandplane. For simplicity, the $z$ axis is assumed to pass through the center of the spherical shell. Our imaginary 2D creature cannot visualize the third dimension or a curved 2D surface within it, so the remainder of this discussion is purely abstract for it (similar to us having difficulty in visualizing a 3D curved space in 4D). But since we are 3D creatures, we have the advantage of visualizing the following steps. Fortunately the 2D creature is already familiar with our mathematical constructs, so it can follow our reasoning. With the third axis added, a generic infinitesimal change over _the full_ 3D space corresponds to the distance: $$ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2d\phi^2+dz^2.$$ [image src="gnuastro-figures/sphereandplane.png" text="../gnuastro-figures//sphereandplane.eps"] Figure 9.2: 2D spherical shell (centered on $O$) and flat plane (light gray) tangent to it at point $A$. It is very important to recognize that this change of distance is for _any_ point in the 3D space, not just those changes that occur on the 2D spherical shell of *note Figure 9.2: sphereandplane. Recall that our 2D friend can only do measurements on the 2D surfaces, not the full 3D space. So we have to constrain this general change to any change on the 2D spherical shell. To do that, let’s look at the arbitrary point $P$ on the 2D spherical shell. Its image ($P'$) on the flat plain is also displayed. From the dark gray triangle, we see that $$\sin\theta={r\over R},\quad\cos\theta={R-z\over R}.$$These relations allow the 2D creature to find the value of $z$ (an abstract dimension for it) as a function of r (distance on a flat 2D plane, which it can visualize) and thus eliminate $z$. From $\sin^2\theta+\cos^2\theta=1$, we get $z^2-2Rz+r^2=0$ and solving for $z$, we find: $$z=R\left(1\pm\sqrt{1-{r^2\over R^2}}\right).$$ The $\pm$ can be understood from *note Figure 9.2: sphereandplane.: For each $r$, there are two points on the sphere, one in the upper hemisphere and one in the lower hemisphere. An infinitesimal change in $r$, will create the following infinitesimal change in $z$: $$dz={\mp r\over R}\left(1\over \sqrt{1-{r^2/R^2}}\right)dr.$$Using the positive signed equation instead of $dz$ in the $ds_s^2$ equation above, we get: $$ds_s^2={dr^2\over 1-r^2/R^2}+r^2d\phi^2.$$ The derivation above was done for a spherical shell of radius $R$ as a curved 2D surface. To generalize it to any surface, we can define $K=1/R^2$ as the curvature parameter. Then the general infinitesimal change in a static universe can be written as: $$ds_s^2={dr^2\over 1-Kr^2}+r^2d\phi^2.$$ Therefore, when $K>0$ (and curvature is the same everywhere), we have a finite universe, where $r$ cannot become larger than $R$ as in *note Figure 9.2: sphereandplane. When $K=0$, we have a flat plane (*note Figure 9.1: flatplane.) and a negative $K$ will correspond to an imaginary $R$. The latter two cases may be infinite in area (which is not a simple concept, but mathematically can be modeled with $r$ extending infinitely), or finite-area (like a cylinder is flat everywhere with $ds_s^2={dx^2 + dy^2}$, but finite in one direction in size). A very important issue that can be discussed now (while we are still in 2D and can actually visualize things) is that $\overrightarrow{r}$ is tangent to the curved space at the observer’s position. In other words, it is on the gray flat surface of *note Figure 9.2: sphereandplane, even when the universe if curved: $\overrightarrow{r}=P'-A$. Therefore for the point $P$ on a curved space, the raw coordinate $r$ is the distance to $P'$, not $P$. The distance to the point $P$ (at a specific coordinate $r$ on the flat plane) over the curved surface (thick line in *note Figure 9.2: sphereandplane.) is called the _proper distance_ and is displayed with $l$. For the specific example of *note Figure 9.2: sphereandplane, the proper distance can be calculated with: $l=R\theta$ ($\theta$ is in radians). using the $\sin\theta$ relation found above, we can find $l$ as a function of $r$: $$\theta=\sin^{-1}\left({r\over R}\right)\quad\rightarrow\quad l(r)=R\sin^{-1}\left({r\over R}\right)$$ $R$ is just an arbitrary constant and can be directly found from $K$, so for cleaner equations, it is common practice to set $R=1$, which gives: $l(r)=\sin^{-1}r$. Also note that when $R=1$, then $l=\theta$. Generally, depending on the the curvature, in a _static_ universe the proper distance can be written as a function of the coordinate $r$ as (from now on we are assuming $R=1$): $$l(r)=\sin^{-1}(r)\quad(K>0),\quad\quad l(r)=r\quad(K=0),\quad\quad l(r)=\sinh^{-1}(r)\quad(K<0).$$With $l$, the infinitesimal change of distance can be written in a more simpler and abstract form of $$ds_s^2=dl^2+r^2d\phi^2.$$ Until now, we had assumed a static universe (not changing with time). But our observations so far appear to indicate that the universe is expanding (it isn’t static). Since there is no reason to expect the observed expansion is unique to our particular position of the universe, we expect the universe to be expanding at all points with the same rate at the same time. Therefore, to add a time dependence to our distance measurements, we can include a multiplicative scaling factor, which is a function of time: $a(t)$. The functional form of $a(t)$ comes from the cosmology, the physics we assume for it: general relativity, and the choice of whether the universe is uniform (‘homogeneous’) in density and curvature or inhomogeneous. In this section, the functional form of $a(t)$ is irrelevant, so we can avoid these issues. With this scaling factor, the proper distance will also depend on time. As the universe expands, the distance between two given points will shift to larger values. We thus define a distance measure, or coordinate, that is independent of time and thus doesn’t ‘move’. We call it the _comoving distance_ and display with $\chi$ such that: $l(r,t)=\chi(r)a(t)$. We have therefore, shifted the $r$ dependence of the proper distance we derived above for a static universe to the comoving distance: $$\chi(r)=\sin^{-1}(r)\quad(K>0),\quad\quad \chi(r)=r\quad(K=0),\quad\quad \chi(r)=\sinh^{-1}(r)\quad(K<0).$$ Therefore, $\chi(r)$ is the proper distance to an object at a specific reference time: $t=t_r$ (the $r$ subscript signifies “referenceâ€) when $a(t_r)=1$. At any arbitrary moment ($t\neq{t_r}$) before or after $t_r$, the proper distance to the object can be scaled with $a(t)$. Measuring the change of distance in a time-dependent (expanding) universe only makes sense if we can add up space and time(2). But we can only add bits of space and time together if we measure them in the same units: with a conversion constant (similar to how 1000 is used to convert a kilometer into meters). Experimentally, we find strong support for the hypothesis that this conversion constant is the speed of light (or gravitational waves(3)) in a vacuum. This speed is postulated to be constant(4) and is almost always written as $c$. We can thus parametrize the change in distance on an expanding 2D surface as $$ds^2=c^2dt^2-a^2(t)ds_s^2 = c^2dt^2-a^2(t)(d\chi^2+r^2d\phi^2).$$ ---------- Footnotes ---------- (1) The observations are interpreted under the assumption of uniform curvature. For a relativistic alternative to dark energy (and maybe also some part of dark matter), non-uniform curvature may be even be more critical, but that is beyond the scope of this brief explanation. (2) In other words, making our space-time consistent with Minkowski space-time geometry. In this geometry, different observers at a given point (event) in space-time split up space-time into ‘space’ and ‘time’ in different ways, just like people at the same spatial position can make different choices of splitting up a map into ‘left–right’ and ‘up–down’. This model is well supported by twentieth and twenty-first century observations. (3) The speed of gravitational waves was recently found to be very similar to that of light in vacuum, see arXiv:1710.05834 (https://arxiv.org/abs/1710.05834). (4) In _natural units_, speed is measured in units of the speed of light in vacuum.  File: gnuastro.info, Node: Extending distance concepts to 3D, Next: Invoking astcosmiccal, Prev: Distance on a 2D curved space, Up: CosmicCalculator 9.1.2 Extending distance concepts to 3D --------------------------------------- The concepts of *note Distance on a 2D curved space:: are here extended to a 3D space that _might_ be curved. We can start with the generic infinitesimal distance in a static 3D universe, but this time in spherical coordinates instead of polar coordinates. $\theta$ is shown in *note Figure 9.2: sphereandplane, but here we are 3D beings, positioned on $O$ (the center of the sphere) and the point $O$ is tangent to a 4D-sphere. In our 3D space, a generic infinitesimal displacement will correspond to the following distance in spherical coordinates: $$ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2).$$ Like the 2D creature before, we now have to assume an abstract dimension which we cannot visualize easily. Let’s call the fourth dimension $w$, then the general change in coordinates in the _full_ four dimensional space will be: $$ds_s^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)+dw^2.$$ But we can only work on a 3D curved space, so following exactly the same steps and conventions as our 2D friend, we arrive at: $$ds_s^2={dr^2\over 1-Kr^2}+r^2(d\theta^2+\sin^2{\theta}d\phi^2).$$ In a non-static universe (with a scale factor a(t)), the distance can be written as: $$ds^2=c^2dt^2-a^2(t)[d\chi^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)].$$  File: gnuastro.info, Node: Invoking astcosmiccal, Prev: Extending distance concepts to 3D, Up: CosmicCalculator 9.1.3 Invoking CosmicCalculator ------------------------------- CosmicCalculator will calculate cosmological variables based on the input parameters. The executable name is ‘astcosmiccal’ with the following general template $ astcosmiccal [OPTION...] ... One line examples: ## Print basic cosmological properties at redshift 2.5: $ astcosmiccal -z2.5 ## Only print Comoving volume over 4pi stradian to z (Mpc^3): $ astcosmiccal --redshift=0.8 --volume ## Print luminosity distance, angular diameter distance and age ## of universe in one row at redshift 0.4 $ astcosmiccal -z0.4 -LAg ## Assume Lambda and matter density of 0.7 and 0.3 and print ## basic cosmological parameters for redshift 2.1: $ astcosmiccal -l0.7 -m0.3 -z2.1 The input parameters (for example current matter density and etc) can be given as command-line options or in the configuration files, see *note Configuration files::. For a definition of the different parameters, please see the sections prior to this. If no redshift is given, CosmicCalculator will just print its input parameters and abort. For a full list of the input options, please see *note CosmicCalculator input options::. When only a redshift is given, CosmicCalculator will print all calculations (one per line) with some explanations before each. This can be good when you want a general feeling of the conditions at a specific redshift. Alternatively, if any specific calculations are requested, only the requested values will be calculated and printed with one character space between them. In this case, no description will be printed. See *note CosmicCalculator specific calculations:: for the full list of these options along with some explanations how when/how they can be useful. * Menu: * CosmicCalculator input options:: Options to specify input conditions. * CosmicCalculator specific calculations:: Requesting specific outputs.  File: gnuastro.info, Node: CosmicCalculator input options, Next: CosmicCalculator specific calculations, Prev: Invoking astcosmiccal, Up: Invoking astcosmiccal 9.1.3.1 CosmicCalculator input options ...................................... The inputs to CosmicCalculator can be specified with the following options: ‘-z FLT’ ‘--redshift=FLT’ The redshift of interest. ‘-H FLT’ ‘--H0=FLT’ Current expansion rate (in km sec$^{-1}$ Mpc$^{-1}$). ‘-l FLT’ ‘--olambda=FLT’ Cosmological constant density divided by the critical density in the current Universe ($\Omega_{\Lambda,0}$). ‘-m FLT’ ‘--omatter=FLT’ Matter (including massive neutrinos) density divided by the critical density in the current Universe ($\Omega_{m,0}$). ‘-r FLT’ ‘--oradiation=FLT’ Radiation density divided by the critical density in the current Universe ($\Omega_{r,0}$).  File: gnuastro.info, Node: CosmicCalculator specific calculations, Prev: CosmicCalculator input options, Up: Invoking astcosmiccal 9.1.3.2 CosmicCalculator specific calculations .............................................. By default, when no specific calculations are requested, CosmicCalculator will print a complete set of all its calculators (one line for each calculation, see *note Invoking astcosmiccal::). The full list of calculations can be useful when you don’t want any specific value, but just a general view. In other contexts (for example in a batch script or during a discussion), you know exactly what you want and don’t want to be distracted by all the extra information. You can use any number of the options described below in any order. When any of these options are requested, CosmicCalculator’s output will just be a single line with a single space between the (possibly) multiple values. In the example below, only the tangential distance along one arcsecond (in kpc), absolute magnitude conversion, and age of the universe at redshift 2 are printed (recall that you can merge short options together, see *note Options::). $ astcosmiccal -z2 -sag 8.585046 44.819248 3.289979 Here is one example of using this feature in scripts: by adding the following two lines in a script to keep/use the comoving volume with varying redshifts: z=3.12 vol=$(astcosmiccal --redshift=$z --volume) In a script, this operation might be necessary for a large number of objects (several of galaxies in a catalog for example). So the fact that all the other default calculations are ignored will also help you get to your result faster. If you are indeed dealing with many (for example thousands) of redshifts, using CosmicCalculator is not the best/fastest solution. Because it has to go through all the configuration files and preparations for each invocation. To get the best efficiency (least overhead), we recommend using Gnuastro’s cosmology library (see *note Cosmology library::). CosmicCalculator also calls the library functions defined there for its calculations, so you get the same result with no overhead. Gnuastro also has libraries for easily reading tables into a C program, see *note Table input output::. Afterwards, you can easily build and run your C program for the particular processing with *note BuildProgram::. If you just want to inspect the value of a variable visually, the description (which comes with units) might be more useful. In such cases, the following command might be better. The other calculations will also be done, but they are so fast that you will not notice on modern computers (the time it takes your eye to focus on the result is usually longer than the processing: a fraction of a second). $ astcosmiccal --redshift=0.832 | grep volume The full list of CosmicCalculator’s specific calculations is present below. In case you have forgot the units, you can use the ‘--help’ option which has the units along with a short description. ‘-G’ ‘--agenow’ The current age of the universe (given the input parameters) in Giga-years (Gyr). ‘-C’ ‘--criticaldensitynow’ The current critical density (given the input parameters) in grams per centimeter-cube ($g/cm^3$). ‘-d’ ‘--properdistance’ The proper distance (at current time) to object at the given redshift in Megaparsecs (Mpc). See *note Distance on a 2D curved space:: for a description of the proper distance. ‘-A’ ‘--angulardimdist’ The angular diameter distance to object at given redshift in Megaparsecs (Mpc). ‘-s’ ‘--arcsectandist’ The tangential distance covered by 1 arcseconds at the given redshift in kiloparsecs (Kpc). This can be useful when trying to estimate the resolution or pixel scale of an instrument (usually in units of arcseconds) at a given redshift. ‘-L’ ‘--luminositydist’ The luminosity distance to object at given redshift in Megaparsecs (Mpc). ‘-u’ ‘--distancemodulus’ The distance modulus at given redshift. ‘-a’ ‘--absmagconv’ The conversion factor (addition) to absolute magnitude. Note that this is practically the distance modulus added with $-2.5\log{(1+z)}$ for the the desired redshift based on the input parameters. Once the apparent magnitude and redshift of an object is known, this value may be added with the apparent magnitude to give the object’s absolute magnitude. ‘-g’ ‘--age’ Age of the universe at given redshift in Giga-years (Gyr). ‘-b’ ‘--lookbacktime’ The look-back time to given redshift in Giga-years (Gyr). The look-back time at a given redshift is defined as the current age of the universe (‘--agenow’) subtracted by the age of the universe at the given redshift. ‘-c’ ‘--criticaldensity’ The critical density at given redshift in grams per centimeter-cube ($g/cm^3$). ‘-v’ ‘--onlyvolume’ The comoving volume in Megaparsecs cube (Mpc$^3$) until the desired redshift based on the input parameters.  File: gnuastro.info, Node: Library, Next: Developing, Prev: High-level calculations, Up: Top 10 Library ********** Each program in Gnuastro that was discussed in the prior chapters (or any program in general) is a collection of functions that is compiled into one executable file which can communicate directly with the outside world. The outside world in this context is the operating system. By communication, we mean that control is directly passed to a program from the operating system with a (possible) set of inputs and after it is finished, the program will pass control back to the operating system. For programs written in C and C++, the unique ‘main’ function is in charge of this communication. Similar to a program, a library is also a collection of functions that is compiled into one executable file. However, unlike programs, libraries don’t have a ‘main’ function. Therefore they can’t communicate directly with the outside world. This gives you the chance to write your own ‘main’ function and call library functions from within it. After compiling your program into a binary executable, you just have to _link_ it to the library and you are ready to run (execute) your program. In this way, you can use Gnuastro at a much lower-level, and in combination with other libraries on your system, you can significantly boost your creativity. This chapter starts with a basic introduction to libraries and how you can use them in *note Review of library fundamentals::. The separate functions in the Gnuastro library are then introduced (classified by context) in *note Gnuastro library::. If you end up routinely using a fixed set of library functions, with a well-defined input and output, it will be much more beneficial if you define a program for the job. Therefore, in its *note Version controlled source::, Gnuastro comes with the *note The TEMPLATE program:: to easily define your own programs(s). * Menu: * Review of library fundamentals:: Guide on libraries and linking. * BuildProgram:: Link and run source files with this library. * Gnuastro library:: Description of all library functions. * Library demo programs:: Demonstration for using libraries.  File: gnuastro.info, Node: Review of library fundamentals, Next: BuildProgram, Prev: Library, Up: Library 10.1 Review of library fundamentals =================================== Gnuastro’s libraries are written in the C programming language. In *note Why C::, we have thoroughly discussed the reasons behind this choice. C was actually created to write Unix, thus understanding the way C works can greatly help in effectively using programs and libraries in all Unix-like operating systems. Therefore, in the following subsections some important aspects of C, as it relates to libraries (and thus programs that depend on them) on Unix are reviewed. First we will discuss header files in *note Headers:: and then go onto *note Linking::. This section finishes with *note Summary and example on libraries::. If you are already familiar with these concepts, please skip this section and go directly to *note Gnuastro library::. In theory, a full operating system (or any software) can be written as one function. Such a software would not need any headers or linking (that are discussed in the subsections below). However, writing that single function and maintaining it (adding new features, fixing bugs, documentation and etc) would be a programmer or scientist’s worst nightmare! Furthermore, all the hard work that went into creating it cannot be reused in other software: every other programmer or scientist would have to re-invent the wheel. The ultimate purpose behind libraries (which come with headers and have to be linked) is to address this problem and increase modularity: “the degree to which a system’s components may be separated and recombined†(from Wikipedia). The more modular the source code of a program or library, the easier maintaining it will be, and all the hard work that went into creating it can be reused for a wider range of problems. * Menu: * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries.  File: gnuastro.info, Node: Headers, Next: Linking, Prev: Review of library fundamentals, Up: Review of library fundamentals 10.1.1 Headers -------------- C source code is read from top to bottom in the source file, therefore program components (for example variables, data structures and functions) should all be _defined_ or _declared_ closer to the top of the source file: before they are used. _Defining_ something in C or C++ is jargon for providing its full details. _Declaring_ it, on the other-hand, is jargon for only providing the minimum information needed for the compiler to pass it temporarily and fill in the detailed definition later. For a function, the _declaration_ only contains the inputs and their data-types along with the output’s type(1). The _definition_ adds to the declaration by including the exact details of what operations are done to the inputs to generate the output. As an example, take this simple summation function: double sum(double a, double b) { return a + b; } What you see above is the _definition_ of this function: it shows you (and the compiler) exactly what it does to the two ‘double’ type inputs and that the output also has a ‘double’ type. Note that a function’s internal operations are rarely so simple and short, it can be arbitrarily long and complicated. This unreasonably short and simple function was chosen here for ease of reading. The declaration for this function is: double sum(double a, double b); You can think of a function’s declaration as a building’s address in the city, and the definition as the building’s complete blueprints. When the compiler confronts a call to a function during its processing, it doesn’t need to know anything about how the inputs are processed to generate the output. Just as the postman doesn’t need to know the inner structure of a building when delivering the mail. The declaration (address) is enough. Therefore by _declaring_ the functions once at the start of the source files, we don’t have to worry about _defining_ them after they are used. Even for a simple real-world operation (not a simple summation like above!), you will soon need many functions (for example, some for reading/preparing the inputs, some for the processing, and some for preparing the output). Although it is technically possible, managing all the necessary functions in one file is not easy and is contrary to the modularity principle (see *note Review of library fundamentals::), for example the functions for preparing the input can be usable in your other projects with a different processing. Therefore, as we will see later (in *note Linking::), the functions don’t necessarily need to be defined in the source file where they are used. As long as their definitions are ultimately linked to the final executable, everything will be fine. For now, it is just important to remember that the functions that are called within one source file must be declared within the source file (declarations are mandatory), but not necessarily defined there. In the spirit of modularity, it is common to define contextually similar functions in one source file. For example, in Gnuastro, functions that calculate the median, mean and other statistical functions are defined in ‘lib/statistics.c’, while functions that deal directly with FITS files are defined in ‘lib/fits.c’. Keeping the definition of similar functions in a separate file greatly helps their management and modularity, but this fact alone doesn’t make things much easier for the caller’s source code: recall that while definitions are optional, declarations are mandatory. So if this was all, the caller would have to manually copy and paste (_include_) all the declarations from the various source files into the file they are working on now. To address this problem, programmers have adopted the header file convention: the header file of a source code contains all the declarations that a caller would need to be able to use any of its functions. For example, in Gnuastro, ‘lib/statistics.c’ (file containing function definitions) comes with ‘lib/gnuastro/statistics.h’ (only containing function declarations). The discussion above was mainly focused on functions, however, there are many more programming constructs such as pre-processor macros and data structures. Like functions, they also need to be known to the compiler when it confronts a call to them. So the header file also contains their definitions or declarations when they are necessary for the functions. Pre-processor macros (or macros for short) are replaced with their defined value by the pre-processor before compilation. Conventionally they are written only in capital letters to be easily recognized. It is just important to understand that the compiler doesn’t see the macros, it sees their fixed values. So when a header specifies macros you can do your programming without worrying about the actual values. The standard C types (for example ‘int’, or ‘float’) are very low-level and basic. We can collect multiple C types into a _structure_ for a higher-level way to keep and pass-along data. See *note Generic data container:: for some examples of macros and data structures. The contents in the header need to be _include_d into the caller’s source code with a special pre-processor command: ‘#include ’. As the name suggests, the _pre-processor_ goes through the source code prior to the processor (or compiler). One of its jobs is to include, or merge, the contents of files that are mentioned with this directive in the source code. Therefore the compiler sees a single entity containing the contents of the main file and all the included files. This allows you to include many (sometimes thousands of) declarations into your code with only one line. Since the headers are also installed with the library into your system, you don’t even need to keep a copy of them for each separate program, making things even more convenient. Try opening some of the ‘.c’ files in Gnuastro’s ‘lib/’ directory with a text editor to check out the include directives at the start of the file (after the copyright notice). Let’s take ‘lib/fits.c’ as an example. You will notice that Gnuastro’s header files (like ‘gnuastro/fits.h’) are indeed within this directory (the ‘fits.h’ file is in the ‘gnuastro/’ directory). You will notice that files like ‘stdio.h’, or ‘string.h’ are not in this directory (or anywhere within Gnuastro). On most systems the basic C header files (like ‘stdio.h’ and ‘string.h’ mentioned above) are located in ‘/usr/include/’(2). Your compiler is configured to automatically search that directory (and possibly others), so you don’t have to explicitly mention these directories. Go ahead, look into the ‘/usr/include’ directory and find ‘stdio.h’ for example. When the necessary header files are not in those specific libraries, the pre-processor can also search in places other than the current directory. You can specify those directories with this pre-processor option(3): ‘-I DIR’ “Add the directory ‘DIR’ to the list of directories to be searched for header files. Directories named by ’-I’ are searched before the standard system include directories. If the directory ‘DIR’ is a standard system include directory, the option is ignored to ensure that the default search order for system directories and the special treatment of system headers are not defeated...†(quoted from the GNU Compiler Collection manual). Note that the space between and the directory is optional and commonly not used. If the pre-processor can’t find the included files, it will abort with an error. In fact a common error when building programs that depend on a library is that the compiler doesn’t not know where a library’s header is (see *note Known issues::). So you have to manually tell the compiler where to look for the library’s headers with the ‘-I’ option. For a small software with one or two source files, this can be done manually (see *note Summary and example on libraries::). However, to enhance modularity, Gnuastro (and most other bin/libraries) contain many source files, so the compiler is invoked many times(4). This makes manual addition or modification of this option practically impossible. To solve this problem, in the GNU build system, there are conventional environment variables for the various kinds of compiler options (or flags). These environment variables are used in every call to the compiler (they can be empty). The environment variable used for the C Pre-Processor (or CPP) is ‘CPPFLAGS’. By giving ‘CPPFLAGS’ a value once, you can be sure that each call to the compiler will be affected. See *note Known issues:: for an example of how to set this variable at configure time. As described in *note Installation directory::, you can select the top installation directory of a software using the GNU build system, when you ‘./configure’ it. All the separate components will be put in their separate sub-directory under that, for example the programs, compiled libraries and library headers will go into ‘$prefix/bin’ (replace ‘$prefix’ with a directory), ‘$prefix/lib’, and ‘$prefix/include’ respectively. For enhanced modularity, libraries that contain diverse collections of functions (like GSL, WCSLIB, and Gnuastro), put their header files in a sub-directory unique to themselves. For example all Gnuastro’s header files are installed in ‘$prefix/include/gnuastro’. In your source code, you need to keep the library’s sub-directory when including the headers from such libraries, for example ‘#include ’(5). Not all libraries need to follow this convention, for example CFITSIO only has one header (‘fitsio.h’) which is directly installed in ‘$prefix/include’. ---------- Footnotes ---------- (1) Recall that in C, functions only have one output. (2) The ‘include/’ directory name is taken from the pre-processor’s ‘#include’ directive, which is also the motivation behind the ‘I’ in the ‘-I’ option to the pre-processor. (3) Try running Gnuastro’s ‘make’ and find the directories given to the compiler with the ‘-I’ option. (4) Nearly every command you see being executed after running ‘make’ is one call to the compiler. (5) the top ‘$prefix/include’ directory is usually known to the compiler  File: gnuastro.info, Node: Linking, Next: Summary and example on libraries, Prev: Headers, Up: Review of library fundamentals 10.1.2 Linking -------------- To enhance modularity, similar functions are defined in one source file (with a ‘.c’ suffix, see *note Headers:: for more). After running ‘make’, each human-readable, ‘.c’ file is translated (or compiled) into a computer-readable “object†file (ending with ‘.o’). Note that object files are also created when building programs, they aren’t particular to libraries. Try opening Gnuastro’s ‘lib/’ and ‘bin/progname/’ directories after running ‘make’ to see these object files(1). Afterwards, the object files are _linked_ together to create an executable program or a library. The object files contain the full definition of the functions in the respective ‘.c’ file along with a list of any other function (or generally “symbolâ€) that is referenced there. To get a list of those functions you can use the ‘nm’ program which is part of GNU Binutils. For example from the top Gnuastro directory, run: $ nm bin/arithmetic/arithmetic.o This will print a list of all the functions (more generally, ‘symbols’) that were called within ‘bin/arithmetic/arithmetic.c’ along with some further information (for example a ‘T’ in the second column shows that this function is actually defined here, ‘U’ says that it is undefined here). Try opening the ‘.c’ file to check some of these functions for your self. Run ‘info nm’ for more information. To recap, the _compiler_ created the separate object files mentioned above for each ‘.c’ file. The _linker_ will then combine all the symbols of the various object files (and libraries) into one program or library. In the case of Arithmetic (a program) the contents of the object files in ‘bin/arithmetic/’ are copied (and re-ordered) into one final executable file which we can run from the operating system. When the symbols (computer-readable function definitions in most cases) are copied into the output like this, we call the process _static_ linking. Let’s have a closer look at static linking: we’ll assume you have installed Gnuastro into the default ‘/usr/local/’ directory (see *note Installation directory::). If you tried the ‘nm’ command on one of Arithmetic’s object files above, then with the command below you can confirm that all the functions that were defined in the object files (had a ‘T’ in the second column) are also defined in the ‘astarithmetic’ executable: $ nm /usr/local/bin/astarithmetic But you will notice that there are still many undefined symbols (have a ‘U’ in the second column). One class of such functions are Gnuastro’s own library functions that start with ‘‘gal_’’: $ nm /usr/local/bin/astarithmetic | grep gal_ These undefined symbols (functions) will be linked to the executable every time you run arithmetic. Therefore they are known as dynamically _linked_ libraries (2). When the functions of a library need to be dynamically linked, the library is known as a shared library. As we saw above, static linking is done when the executable is being built. However, when a library is linked dynamically, its symbols are only checked with the available libraries at build time: they are not actually copied into the executable. Every time you run the program, the linker will be activated and will try to link the program to the installed library before it starts. If you want all the libraries to be statically linked to the executables, you have to tell Libtool (which Gnuastro uses for the linking) to disable shared libraries at configure time(3): $ configure --disable-shared Try configuring, statically building and installing Gnuastro with the command above. Then check the ‘gal_’ symbols in the installed Arithmetic executable like before. You will see that they are actually copied this time (have a ‘T’ in the second column). If the second column doesn’t convince you, look at the executable file size with the following command: $ ls -lh /usr/local/bin/astarithmetic It should be around 4.2 Megabytes with this static linking. If you configure and build Gnuastro again with shared libraries enabled (which is the default), you will notice that it is roughly 100 Kilobytes! This huge difference would have been very significant in the old days, but with the roughly Terabyte storage drives commonly in use today, it is negligible. Fortunately, output file size is not the only benefit of dynamic linking: since it links to the libraries at run-time (rather than build-time), you don’t have to re-build a higher-level program or library when an update comes for one of the lower-level libraries it depends on. You just install the new low-level library and it will automatically be used next time in your higher-level tools. To be fair, this also creates a few complications(4): • Reproducibility: Even though your high-level tool has the same version as before, with the updated library, you might not get the same results. • Broken links: if some functions have been changed or removed in the updated library, then the linker will abort with an error at run-time. Therefore you need to re-build your higher-level program or library. To see a list of all the shared libraries that are needed for a program or a shared library to run, you can use the GNU C library’s ‘ldd’(5) program, for example: $ ldd /usr/local/bin/astarithmetic Library file names start with a ‘lib’ and end with suffix depending on their type as described below. In between these two is the name of the library, for example ‘libgnuastro.a’ (Gnuastro’s static library) and ‘libgsl.so.0.0.0’ (GSL’s shared library). • A static library is known as an archive file and has a ‘.a’ suffix. A static library is not an executable file. • A shared library ends with a ‘.so.X.Y.Z’ suffix and is executable. The three numbers in the prefix are the version of the shared library. Shared library versions are defined to allow multiple versions of a shared library simultaneously on a system and to help detect possible updates in the library and programs that depend on it by the linker. It is very important to mention that this version number is different from from the software version number (see *note Version numbering::), so do not confuse the two. See the “Library interface versions†chapter of GNU Libtool for more. For each shared library, we also have two symbolic links ending with ‘.so.X’ and ‘.so’. They are automatically set by the installer, but you can change them (point them to another version of the library) when you have multiple versions on your system. For those libraries that use GNU Libtool (including Gnuastro and its dependencies), both static and dynamic libraries are built and installed in the ‘prefix/lib/’ directory (see *note Installation directory::). In this way other programs can make which ever kind of link that they want. To link with a library, the linker needs to know where to find the library. You do that with two separate options to the linker (see *note Summary and example on libraries:: for an example): ‘-L DIR’ Will tell the linker to look into ‘DIR’ for the libraries. For example ‘-L/usr/local/lib’, or ‘-L/home/yourname/.local/lib’. You can make multiple calls to this option, so the linker looks into several directories. Note that the space between and the directory is optional and commonly not used. ‘-lLIBRARY’ Specify the unique name of a library to be linked. As discussed above, library file names have fixed parts which must not be given to this option. So ‘-lgsl’ will guide the linker to either look for ‘libgsl.a’ or ‘libgsl.so’ (depending on the type of linking it is suppose to do). You can link many libraries by repeated calls to this option. *Very important: * The place of this option on the command line matters. This is often a source of confusion for beginners, so let’s assume you have asked the linker to link with library A using this option. As soon as the linker confronts this option, it looks into the list of the undefined symbols it has found until that point and does a search in library A for any of those symbols. If any pending undefined symbol is found in library A, it is used. After the search in undefined symbols is complete, the contents of library A are completely discarded from the linker’s memory. Therefore, if a later object file or library uses an unlinked symbol in library A, the linker will abort after it has finished its search in all the input libraries or object files. As an example, Gnuastro’s ‘gal_array_dlog10_array’ function depends on the ‘log10’ function of the C Math library (specified with ‘-lm’). So the proper way to link something that uses this function is ‘-lgnuastro -lm’. If instead, you give: ‘-lm -lgnuastro’ the linker will complain and abort. ---------- Footnotes ---------- (1) Gnuastro uses GNU Libtool for portable library creation. Libtool will also make a ‘.lo’ file for each ‘.c’ file when building libraries (‘.lo’ files are human-readable). (2) Do not confuse dynamically _linked_ libraries with dynamically _loaded_ libraries. The former (that is discussed here) are only loaded once at the program startup. However, the latter can be loaded anytime during the program’s execution, they are also known as plugins. (3) Libtool is very common and is commonly used. Therefore, you can use this option to configure on most programs using the GNU build system if you want static linking. (4) Both of these can be avoided by joining the mailing lists of the lower-level libraries and checking the changes in newer versions before installing them. Updates that result in such behaviors are generally heavily emphasized in the release notes. (5) If your operating system is not using the GNU C library, you might need another tool.  File: gnuastro.info, Node: Summary and example on libraries, Prev: Linking, Up: Review of library fundamentals 10.1.3 Summary and example on libraries --------------------------------------- After the mostly abstract discussions of *note Headers:: and *note Linking::, we’ll give a small tutorial here. But before that, let’s recall the general steps of how your source code is prepared, compiled and linked to the libraries it depends on so you can run it: 1. The *pre-processor* includes the header (‘.h’) files into the function definition (‘.c’) files, expands pre-processor macros and generally prepares the human-readable source for compilation (reviewed in *note Headers::). 2. The *compiler* will translate (compile) the human-readable contents of each source (merged ‘.c’ and the ‘.h’ files, or generally the output of the pre-processor) into the computer-readable code of ‘.o’ files. 3. The *linker* will link the called function definitions from various compiled files to create one unified object. When the unified product has a ‘main’ function, this function is the product’s only entry point, enabling the operating system or user to directly interact with it, so the product is a program. When the product doesn’t have a ‘main’ function, the linker’s product is a library and its exported functions can be linked to other executables (it has many entry points). The GNU Compiler Collection (or GCC for short) will do all three steps. So as a first example, from Gnuastro’s source, go to ‘tests/lib/’. This directory contains the library tests, you can use these as some simple tutorials. For this demonstration, we will compile and run the ‘arraymanip.c’. This small program will call Gnuastro library for some simple operations on an array (open it and have a look). To compile this program, run this command inside the directory containing it. $ gcc arraymanip.c -lgnuastro -lm -o arraymanip The two ‘-lgnuastro’ and ‘-lm’ options (in this order) tell GCC to first link with the Gnuastro library and then with C’s math library. The ‘-o’ option is used to specify the name of the output executable, without it the output file name will be ‘a.out’ (on most OSs), independent of your input file name(s). If your top Gnuastro installation directory (let’s call it ‘$prefix’, see *note Installation directory::) is not recognized by GCC, you will get pre-processor errors for unknown header files. Once you fix it, you will get linker errors for undefined functions. To fix both, you should run GCC as follows: additionally telling it which directories it can find Gnuastro’s headers and compiled library (see *note Headers:: and *note Linking::): $ gcc -I$prefix/include -L$prefix/lib arraymanip.c -lgnuastro -lm \ -o arraymanip This single command has done all the pre-processor, compilation and linker operations. Therefore no intermediate files (object files in particular) were created, only a single output executable was created. You are now ready to run the program with: $ ./arraymanip The Gnuastro functions called by this program only needed to be linked with the C math library. But if your program needs WCS coordinate transformations, needs to read a FITS file, needs special math operations (which include its linear algebra operations), or you want it to run on multiple CPU threads, you also need to add these libraries in the call to GCC: ‘-lgnuastro -lwcs -lcfitsio -lgsl -lgslcblas -pthread -lm’. In *note Gnuastro library::, where each function is documented, it is mentioned which libraries (if any) must also be linked when you call a function. If you feel all these linkings can be confusing, please consider Gnuastro’s *note BuildProgram:: program.  File: gnuastro.info, Node: BuildProgram, Next: Gnuastro library, Prev: Review of library fundamentals, Up: Library 10.2 BuildProgram ================= The number and order of libraries that are necessary for linking a program with Gnuastro library might be too confusing when you need to compile a small program for one particular job (with one source file). BuildProgram will use the information gathered during configuring Gnuastro and link with all the appropriate libraries on your system. This will allow you to easily compile, link and run programs that use Gnuastro’s library with one simple command and not worry about which libraries to link to, or the linking order. BuildProgram uses GNU Libtool to find the necessary libraries to link against (GNU Libtool is the same program that builds all of Gnuastro’s libraries and programs when you run ‘make’). So in the future, if Gnuastro’s prerequisite libraries change or other libraries are added, you don’t have to worry, you can just run BuildProgram and internal linking will be done correctly. *BuildProgram requires GNU Libtool:* BuildProgram depends on GNU Libtool, other implementations don’t have some necessary features. If GNU Libtool isn’t available at Gnuastro’s configure time, you will get a notice at the end of the configuration step and BuildProgram will not be built or installed. Please see *note Optional dependencies:: for more information. * Menu: * Invoking astbuildprog:: Options and examples for using this program.  File: gnuastro.info, Node: Invoking astbuildprog, Prev: BuildProgram, Up: BuildProgram 10.2.1 Invoking BuildProgram ---------------------------- BuildProgram will compile and link a C source program with Gnuastro’s library and all its dependencies, greatly facilitating the compilation and running of small programs that use Gnuastro’s library. The executable name is ‘astbuildprog’ with the following general template: $ astbuildprog [OPTION...] C_SOURCE_FILE One line examples: ## Compile, link and run `myprogram.c': $ astbuildprog myprogram.c ## Similar to previous, but with optimization and compiler warnings: $ astbuildprog -Wall -O2 myprogram.c ## Compile and link `myprogram.c', then run it with `image.fits' ## as its argument: $ astbuildprog myprogram.c image.fits ## Also look in other directories for headers and linking: $ astbuildprog -Lother -Iother/dir myprogram.c ## Just build (compile and link) `myprogram.c', don't run it: $ astbuildprog --onlybuild myprogram.c If BuildProgram is to run, it needs a C programming language source file as input. By default it will compile and link the program to build the a final executable file and run it. The built executable name can be set with the optional ‘--output’ option. When no output name is set, BuildProgram will use Gnuastro’s *note Automatic output::, and remove the suffix of the input and use that as the output name. For the full list of options that BuildProgram shares with other Gnuastro programs, see *note Common options::. You may also use Gnuastro’s *note Configuration files:: to specify other libraries/headers to use for special directories and not have to type them in every time. The first argument is considered to be the C source file that must be compiled and linked. Any other arguments (non-option tokens on the command-line) will be passed onto the program when BuildProgram wants to run it. Recall that by default BuildProgram will run the program after building it. This behavior can be disabled with the ‘--onlybuild’ option. When the ‘--quiet’ option (see *note Operating mode options::) is not called, BuildPrograms will print the compilation and running commands. Once your program grows and you break it up into multiple files (which are much more easily managed with Make), you can use the linking flags of the non-quiet output in your ‘Makefile’. ‘-I STR’ ‘--includedir=STR’ Directory to search for files that you ‘#include’ in your C program. Note that headers relating to Gnuastro and its dependencies don’t need this option. This is only necessary if you want to use other headers. It may be called multiple times and order matters. This directory will be searched before those of Gnuastro’s build and also the system search directories. See *note Headers:: for a thorough introduction. From the GNU C Pre-Processor manual: “Add the directory ‘STR’ to the list of directories to be searched for header files. Directories named by ‘-I’ are searched before the standard system include directories. If the directory ‘STR’ is a standard system include directory, the option is ignored to ensure that the default search order for system directories and the special treatment of system headers are not defeatedâ€. ‘-L STR’ ‘--linkdir=STR’ Directory to search for compiled libraries to link the program with. Note that all the directories that Gnuastro was built with will already be used by BuildProgram (GNU Libtool). This option is only necessary if your libraries are in other directories. Multiple calls to this option are possible and order matters. This directory will be searched before those of Gnuastro’s build and also the system search directories. See *note Linking:: for a thorough introduction. ‘-l STR’ ‘--linklib=STR’ Library to link with your program. Note that all the libraries that Gnuastro was built with will already be linked by BuildProgram (GNU Libtool). This option is only necessary if you want to link with other directories. Multiple calls to this option are possible and order matters. This library will be linked before Gnuastro’s library or its dependencies. See *note Linking:: for a thorough introduction. ‘-O INT/STR’ ‘--optimize=INT/STR’ Compiler optimization level: 0 (for no optimization, good debugging), 1, 2, 3 (for the highest level of optimizations). From the GNU Compiler Collection (GCC) manual: “Without any optimization option, the compiler’s goal is to reduce the cost of compilation and to make debugging produce the expected results. Statements are independent: if you stop the program with a break point between statements, you can then assign a new value to any variable or change the program counter to any other statement in the function and get exactly the results you expect from the source code. Turning on optimization flags makes the compiler attempt to improve the performance and/or code size at the expense of compilation time and possibly the ability to debug the program.†Please see your compiler’s manual for the full list of acceptable values to this option. ‘-g’ ‘--debug’ Emit extra information in the compiled binary for use by a debugger. When calling this option, it is best to explicitly disable optimization with ‘-O0’. To combine both options you can run ‘-gO0’ (see *note Options:: for how short options can be merged into one). ‘-W STR’ ‘--warning=STR’ Print compiler warnings on command-line during compilation. “Warnings are diagnostic messages that report constructions that are not inherently erroneous but that are risky or suggest there may have been an error.†(from the GCC manual). It is always recommended to compile your programs with warnings enabled. All compiler warning options that start with ‘W’ are usable by this option in BuildProgram also, see your compiler’s manual for the full list. Some of the most common values to this option are: ‘pedantic’ (Warnings related to standard C) and ‘all’ (all issues the compiler confronts). ‘--tag=STR’ The language configuration information. Libtool can build objects and libraries in many languages. In many cases, it can identify the language automatically, but when it doesn’t you can use this option to explicitly notify Libtool of the language. The acceptable values are: ‘CC’ for C, ‘CXX’ for C++, ‘GCJ’ for Java, ‘F77’ for Fortran 77, ‘FC’ for Fortran, ‘GO’ for Go and ‘RC’ for Windows Resource. Note that the Gnuastro library is not yet fully compatible with all these languages. ‘-b’ ‘--onlybuild’ Only build the program, don’t run it. By default, the built program is immediately run afterwards. ‘--deletecompiled’ Delete the compiled binary file after running it. This option is only relevant when the compiled program is run after being built. In other words, it is only relevant when ‘--onlybuild’ is not called. It can be useful when you are busy testing a program or just want a fast result and the actual binary/compiled file is not of later use. ‘-a STR’ ‘--la=STR’ Use the given ‘.la’ file (Libtool control file) instead of the one that was produced from Gnuastro’s configuration results. The Libtool control file keeps all the necessary information for building and linking a program with a library built by Libtool. The default ‘prefix/lib/libgnuastro.la’ keeps all the information necessary to build a program using the Gnuastro library gathered during configure time (see *note Installation directory:: for prefix). This option is useful when you prefer to use another Libtool control file.  File: gnuastro.info, Node: Gnuastro library, Next: Library demo programs, Prev: BuildProgram, Up: Library 10.3 Gnuastro library ===================== Gnuastro library’s programming constructs (function declarations, macros, data structures, or global variables) are classified by context into multiple header files (see *note Headers::)(1). In this section, the functions in each header will be discussed under a separate sub-section, which includes the name of the header. Assuming a function declaration is in ‘headername.h’, you can include its declaration in your source code with: # include The names of all constructs in ‘headername.h’ are prefixed with ‘gal_headername_’ (or ‘GAL_HEADERNAME_’ for macros). The ‘gal_’ prefix stands for _G_NU _A_stronomy _L_ibrary. Gnuastro library functions are compiled into a single file which can be linked on the command-line with the ‘-lgnuastro’ option, (see *note Linking:: and *note Summary and example on libraries:: for an introduction on linking and example). Gnuastro library is a high-level library which depends on lower level libraries for some operations (see *note Dependencies::). Therefore if at least one of Gnuastro’s functions in your program use functions from the dependencies, you will also need to link those dependencies after linking with Gnuastro. The outside libraries that need to be linked for such functions are mentioned following the function name. See *note BuildProgram:: for a small Gnuastro program that will take care of the libraries to link against and lets you focus on your exciting science. *Libraries are still under heavy development: * Gnuastro was initially created to be a collection of command-line programs. However, as the programs and their the shared functions grew, internal (not installed) libraries were added. Since the 0.2 release, the libraries are install-able. Hence the libraries are currently under heavy development and will significantly evolve between releases and will become more mature and stable in due time. It will stabilize with the removal of this notice. Check the ‘NEWS’ file for interface changes. If you use the Info version of this manual (see *note Info::), you don’t have to worry: the documentation will correspond to your installed version. * Menu: * Configuration information:: General information about library config. * Multithreaded programming:: Tools for easy multi-threaded operations. * Library data types:: Definitions and functions for types. * Library blank values:: Blank values and functions to deal with them. * Library data container:: General data container in Gnuastro. * Dimensions:: Dealing with coordinates and dimensions. * Linked lists:: Various types of linked lists. * FITS files:: Working with FITS data. * World Coordinate System:: Dealing with the world coordinate system. * Text files:: Functions to work on Text files. * Table input output:: Reading and writing table columns. * Arithmetic on datasets:: Arithmetic operations on a dataset. * Tessellation library:: Functions for working on tiles. * Bounding box:: Finding the bounding box. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Permutations:: Re-order (or permute) the values in a dataset. * Matching:: Matching catalogs based on position. * Statistical operations:: Functions for basic statistics. * Binary datasets:: Datasets that can only have values of 0 or 1. * Convolution functions:: Library functions to do convolution. * Interpolation:: Interpolate (over blank values possibly). * Git wrappers:: Wrappers for functions in libgit2. * Cosmology library:: Cosmological calculations. ---------- Footnotes ---------- (1) Within Gnuastro’s source, all installed ‘.h’ files in ‘lib/gnuastro/’ are accompanied by a ‘.c’ file in ‘/lib/’.  File: gnuastro.info, Node: Configuration information, Next: Multithreaded programming, Prev: Gnuastro library, Up: Gnuastro library 10.3.1 Configuration information (‘config.h’) --------------------------------------------- The ‘gnuastro/config.h’ header contains information about the full Gnuastro installation on your system. Gnuastro developers should note that this is the only header that is not available within Gnuastro, it is only available to a Gnuastro library user _after_ installation. Within Gnuastro, ‘config.h’ (which is included in every Gnuastro ‘.c’ file, see *note Coding conventions::) has more than enough information about the overall Gnuastro installation. -- Macro: GAL_CONFIG_VERSION This macro can be used as a string literal(1) containing the version of Gnuastro that is being used. See *note Version numbering:: for the version formats. For example: printf("Gnuastro version: %s\n", GAL_CONFIG_VERSION); or char *gnuastro_version=GAL_CONFIG_VERSION; -- Macro: GAL_CONFIG_HAVE_LIBGIT2 Libgit2 is an optional dependency of Gnuastro (see *note Optional dependencies::). When it is installed and detected at configure time, this macro will have a value of ‘1’ (one). Otherwise, it will have a value of ‘0’ (zero). Gnuastro also comes with some wrappers to make it easier to use libgit2 (see *note Git wrappers::). -- Macro: GAL_CONFIG_HAVE_WCSLIB_VERSION WCSLIB is the reference library for world coordinate system transformation (see *note WCSLIB:: and *note World Coordinate System::). However, only more recent versions of WCSLIB also provide its version number. If the WCSLIB that is installed on the system provides its version (through the possibly existing ‘wcslib_version’ function), this macro will have a value of one, otherwise it will have a value of zero. -- Macro: GAL_CONFIG_HAVE_PTHREAD_BARRIER The POSIX threads standard define barriers as an optional requirement. Therefore, some operating systems choose to not include it. As one of the ‘./configure’ step checks, Gnuastro we check if your system has this POSIX thread barriers. If so, this macro will have a value of ‘1’, otherwise it will have a value of ‘0’. see *note Implementation of pthread_barrier:: for more. -- Macro: GAL_CONFIG_SIZEOF_LONG -- Macro: GAL_CONFIG_SIZEOF_SIZE_T The size of (number of bytes in) the system’s ‘long’ and ‘size_t’ types. Their values are commonly either 4 or 8 for 32-bit and 64-bit systems. You can also get this value with the expression ‘‘sizeof size_t’’ for example without having to include this header. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Multithreaded programming, Next: Library data types, Prev: Configuration information, Up: Gnuastro library 10.3.2 Multithreaded programming (‘threads.h’) ---------------------------------------------- In recent years, newer CPUs don’t have significantly higher frequencies any more. However, CPUs are being manufactured with more cores, enabling more than one operation (thread) at each instant. This can be very useful to speed up many aspects of processing and in particular image processing. Most of the programs in Gnuastro utilize multi-threaded programming for the CPU intensive processing steps. This can potentially lead to a significant decrease in the running time of a program, see *note A note on threads::. In terms of reading the code, you don’t need to know anything about multi-threaded programming. You can simply follow the case where only one thread is to be used. In these cases, threads are not used and can be completely ignored. When the C language was defined (the K&R’s book was written), using threads was not common, so C’s threading capabilities aren’t introduced there. Gnuastro uses POSIX threads for multi-threaded programming, defined in the ‘pthread.h’ system wide header. There are various resources for learning to use POSIX threads. An excellent tutorial (https://computing.llnl.gov/tutorials/pthreads/) is provided by the Lawrence Livermore National Laboratory, with abundant figures to better understand the concepts, it is a very good start. The book ‘Advanced programming in the Unix environment’(1), by Richard Stevens and Stephen Rago, Addison-Wesley, 2013 (Third edition) also has two chapters explaining the POSIX thread constructs which can be very helpful. An alternative to POSIX threads was OpenMP, but POSIX threads are low level, allowing much more control, while being easier to understand, see *note Why C::. All the situations where threads are used in Gnuastro currently are completely independent with no need of coordination between the threads. Such problems are known as “embarrassingly parallel†problems. They are some of the simplest problems to solve with threads and are also the ones that benefit most from them, see the LLNL introduction(2). One very useful POSIX thread concept is ‘pthread_barrier’. Unfortunately, it is only an optional feature in the POSIX standard, so some operating systems don’t include it. Therefore in *note Implementation of pthread_barrier::, we introduce our own implementation. This is a rather technical section only necessary for more technical readers and you can safely ignore it. Following that, we describe the helper functions in this header that can greatly simplify writing a multi-threaded program, see *note Gnuastro's thread related functions:: for more. * Menu: * Implementation of pthread_barrier:: Some systems don’t have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. ---------- Footnotes ---------- (1) Don’t let the title scare you! The two chapters on Multi-threaded programming are very self-sufficient and don’t need any more knowledge than K&R. (2)  File: gnuastro.info, Node: Implementation of pthread_barrier, Next: Gnuastro's thread related functions, Prev: Multithreaded programming, Up: Multithreaded programming 10.3.2.1 Implementation of ‘pthread_barrier’ ............................................ One optional feature of the POSIX Threads standard is the ‘pthread_barrier’ concept. It is a very useful high-level construct that allows for independent threads to “wait†behind a “barrier†for the rest after they finish. Barriers can thus greatly simplify the code in a multi-threaded program, so they are heavily used in Gnuastro. However, since its an optional feature in the POSIX standard, some operating systems don’t include it. So to make Gnuastro portable, we have written our own implementation of those ‘pthread_barrier’ functions. At ‘./configure’ time, Gnuastro will check if ‘pthread_barrier’ constructs are available on your system or not. If ‘pthread_barrier’ is not available, our internal implementation will be compiled into the Gnuastro library and the definitions and declarations below will be usable in your code with ‘#include ’. -- Type: pthread_barrierattr_t Type to specify the attributes of a POSIX threads barrier. -- Type: pthread_barrier_t Structure defining the POSIX threads barrier. -- Function: int pthread_barrier_init (pthread_barrier_t ‘*b’, pthread_barrierattr_t ‘*attr’, unsigned int ‘limit’) Initialize the barrier ‘b’, with the attributes ‘attr’ and total ‘limit’ (a number of) threads that must wait behind it. This function must be called before spinning off threads. -- Function: int pthread_barrier_wait (pthread_barrier_t ‘*b’) This function is called within each thread, just before it is ready to return. Once a thread’s function hits this, it will “wait†until all the other functions are also finished. -- Function: int pthread_barrier_destroy (pthread_barrier_t ‘*b’) Destroy all the information in the barrier structure. This should be called by the function that spinned-off the threads after all the threads have finished. *Destroy a barrier before re-using it:* It is very important to destroy the barrier before (possibly) reusing it. This destroy function not only destroys the internal structures, it also waits (in 1 microsecond intervals, so you will not notice!) until all the threads don’t need the barrier structure any more. If you immediately start spinning off new threads with a not-destroyed barrier, then the internal structure of the remaining threads will get mixed with the new ones and you will get very strange and apparently random errors that are extremely hard to debug.  File: gnuastro.info, Node: Gnuastro's thread related functions, Prev: Implementation of pthread_barrier, Up: Multithreaded programming 10.3.2.2 Gnuastro’s thread related functions ............................................ The POSIX Threads functions offered in the C library are very low-level and offer a great range of control over the properties of the threads. So if you are interested in customizing your tools for complicated thread applications, it is strongly encouraged to get a nice familiarity with them. Some resources were introduced in *note Multithreaded programming::. However, in many cases used in astronomical data analysis, you don’t need communication between threads and each target operation can be done independently. Since such operations are very common, Gnuastro provides the tools below to facilitate the creation and management of jobs without any particular knowledge of POSIX Threads for such operations. The most interesting high-level functions of this section are the ‘gal_threads_number’ and ‘gal_threads_spin_off’ that identify the number of threads on the system and spin-off threads. You can see a demonstration of using these functions in *note Library demo - multi-threaded operation::. -- C ‘struct’: gal_threads_params Structure keeping the parameters of each thread. When each thread is created, a pointer to this structure is passed to it. The ‘params’ element can be the pointer to a structure defined by the user which contains all the necessary parameters to pass onto the worker function. The rest of the elements within this structure are set internally by ‘gal_threads_spin_off’ and are relevant to the worker function. struct gal_threads_params { size_t id; /* Id of this thread. */ void *params; /* User-identified pointer. */ size_t *indexs; /* Target indexs given to this thread. */ pthread_barrier_t *b; /* Barrier for all threads. */ }; -- Function: size_t gal_threads_number () Return the number of threads that the operating system has available for your program. This number is usually fixed for a single machine and doesn’t change. So this function is useful when you want to run your program on different machines (with different CPUs). -- Function: void gal_threads_spin_off (void ‘*(*worker)(void *)’, void ‘*caller_params’, size_t ‘numactions’, size_t ‘numthreads’) Distribute ‘numactions’ jobs between ‘numthreads’ threads and spin-off each thread by calling the ‘worker’ function. The ‘caller_params’ pointer will also be passed to ‘worker’ as part of the ‘gal_threads_params’ structure. For a fully working example of this function, please see *note Library demo - multi-threaded operation::. -- Function: void gal_threads_attr_barrier_init (pthread_attr_t ‘*attr’, pthread_barrier_t ‘*b’, size_t ‘limit’) This is a low-level function in case you don’t want to use ‘gal_threads_spin_off’. It will initialize the general thread attribute ‘attr’ and the barrier ‘b’ with ‘limit’ threads to wait behind the barrier. For maximum efficiency, the threads initialized with this function will be detached. Therefore no communication is possible between these threads and in particular ‘pthread_join’ won’t work on these threads. You have to use the barrier constructs to wait for all threads to finish. -- Function: void gal_threads_dist_in_threads (size_t ‘numactions’, size_t ‘numthreads’, size_t ‘**outthrds’, size_t ‘*outthrdcols’) This is a low-level function in case you don’t want to use ‘gal_threads_spin_off’. Identify the “indexâ€es (starting from 0) of the actions to be done on each thread in the ‘outthrds’ array. ‘outthrds’ is treated as a 2D array with ‘numthreads’ rows and ‘outthrdcols’ columns. The indexs in each row, identify the actions that should be done by one thread. Please see the explanation below to understand the purpose of this operation. Let’s assume you have $A$ actions (where there is only one function and the input values differ for each action) and $T$ threads available to the system with $A>T$ (common values for these two would be $A>1000$ and $T<10$). Spinning off a thread is not a cheap job and requires a significant number of CPU cycles. Therefore, creating $A$ threads is not the best way to address such a problem. The most efficient way to manage the actions is such that only $T$ threads are created, and each thread works on a list of actions identified for it in series (one after the other). This way your CPU will get all the actions done with minimal overhead. The purpose of this function is to do what we explained above: each row in the ‘outthrds’ array contains the indexs of actions which must be done by one thread. ‘outthrds’ contains ‘outthrdcols’ columns. In using ‘outthrds’, you don’t have to know the number of columns. The ‘GAL_BLANK_SIZE_T’ macro has a role very similar to a string’s ‘\0’: every row finishes with this macro, so can easily stop parsing the indexes in the row when you confront it. Please see the example program in ‘tests/lib/multithread.c’ for a demonstration.  File: gnuastro.info, Node: Library data types, Next: Library blank values, Prev: Multithreaded programming, Up: Gnuastro library 10.3.3 Library data types (‘type.h’) ------------------------------------ Data in astronomy can have many types, numeric (numbers) and strings (names, identifiers). The former can also be divided into integers and floats, see *note Numeric data types:: for a thorough discussion of the different numeric data types and which one is useful for different contexts. To deal with the very large diversity of types that are available (and used in different contexts), in Gnuastro each type is identified with global integer variable with a fixed name, this variable is then passed onto functions that can work on any type or is stored in Gnuastro’s *note Generic data container:: as one piece of meta-data. The actual values within these integer constants is irrelevant and you should never rely on them. When you need to check, explicitly use the named variable in the table below. If you want to check with more than one type, you can use C’s ‘switch’ statement. Since Gnuastro heavily deals with file input-output, the types it defines are fixed width types, these types are portable to all systems and are defined in the standard C header ‘stdint.h’. You don’t need to include this header, it is included by any Gnuastro header that deals with the different types. However, the most commonly used types in a C (or C++) program (for example ‘int’ or ‘long’ are not defined by their exact width (storage), but by their minimum storage. So for example on some systems, ‘int’ may be 2 bytes (16-bits, the minimum required by the standard) and on others it may be 4 bytes (32-bits, common in modern systems). With every type, a unique “blank†value (or place holder showing the absence of data) can be defined. Please see *note Library blank values:: for constants that Gnuastro recognizes as a blank value for each type. See *note Numeric data types:: for more explanation on the limits and particular aspects of each type. -- Global integer: GAL_TYPE_INVALID This is just a place holder to specifically mark that no type has been set. -- Global integer: GAL_TYPE_BIT Identifier for a bit-stream. Currently no program in Gnuastro works directly on bits, but features will be added in the future. -- Global integer: GAL_TYPE_UINT8 Identifier for an unsigned, 8-bit integer type: ‘uint8_t’ (from ‘stdint.h’), or an ‘unsigned char’ in most modern systems. -- Global integer: GAL_TYPE_INT8 Identifier for a signed, 8-bit integer type: ‘int8_t’ (from ‘stdint.h’), or an ‘signed char’ in most modern systems. -- Global integer: GAL_TYPE_UINT16 Identifier for an unsigned, 16-bit integer type: ‘uint16_t’ (from ‘stdint.h’), or an ‘unsigned short’ in most modern systems. -- Global integer: GAL_TYPE_INT16 Identifier for a signed, 16-bit integer type: ‘int16_t’ (from ‘stdint.h’), or a ‘short’ in most modern systems. -- Global integer: GAL_TYPE_UINT32 Identifier for an unsigned, 32-bit integer type: ‘uint32_t’ (from ‘stdint.h’), or an ‘unsigned int’ in most modern systems. -- Global integer: GAL_TYPE_INT32 Identifier for a signed, 32-bit integer type: ‘int32_t’ (from ‘stdint.h’), or an ‘int’ in most modern systems. -- Global integer: GAL_TYPE_UINT64 Identifier for an unsigned, 64-bit integer type: ‘uint64_t’ (from ‘stdint.h’), or an ‘unsigned long’ in most modern 64-bit systems. -- Global integer: GAL_TYPE_INT64 Identifier for a signed, 64-bit integer type: ‘int64_t’ (from ‘stdint.h’), or an ‘long’ in most modern 64-bit systems. -- Global integer: GAL_TYPE_SIZE_T Identifier for a ‘size_t’ type. This is just an alias to ‘uint32’, or ‘uint64’ types for 32-bit, or 64-bit systems respectively. -- Global integer: GAL_TYPE_LONG Identifier for a ‘long’ type. This is just an alias to ‘int32’, or ‘int64’ types for 32-bit, or 64-bit systems respectively. -- Global integer: GAL_TYPE_FLOAT32 Identifier for a 32-bit single precision floating point type or ‘float’ in C. -- Global integer: GAL_TYPE_FLOAT64 Identifier for a 64-bit double precision floating point type or ‘double’ in C. -- Global integer: GAL_TYPE_COMPLEX32 Identifier for a complex number composed of two ‘float’ types. Note that the complex type is not yet fully implemented in all Gnuastro’s programs. -- Global integer: GAL_TYPE_COMPLEX64 Identifier for a complex number composed of two ‘double’ types. Note that the complex type is not yet fully implemented in all Gnuastro’s programs. -- Global integer: GAL_TYPE_STRING Identifier for a string of characters (‘char *’). -- Global integer: GAL_TYPE_STRLL Identifier for a linked list of string of characters (‘gal_list_str_t’, see *note List of strings::). The functions below are defined to make working with the integer constants above easier. In the functions below, the constants above can be used for the ‘type’ input argument. -- Function: size_t gal_type_sizeof (uint8_t ‘type’) Return the number of bytes occupied by ‘type’. Internally, this function uses C’s ‘sizeof’ operator to measure the size of each type. -- Function: char * gal_type_name (uint8_t ‘type’, int ‘long_name’) Return a string that contains the name of ‘type’. This can be used in messages to the users when your function/program accepts many types. It can return both short and long formats of the type names (for example ‘f32’ and ‘float32’). If ‘long_name’ is non-zero, the long format will be returned, otherwise the short name will be returned. The output string is statically allocated, so it should not be freed. This function is the inverse of the ‘gal_type_from_name’ function. For the full list of names/strings that this function will return, see *note Numeric data types::. -- Function: uint8_t gal_type_from_name (char ‘*str’) Return the Gnuastro integer constant that corresponds to the string ‘str’. This function is the inverse of the ‘gal_type_name’ function and accepts both the short and long formats of each type. For the full list of names/strings that this function will return, see *note Numeric data types::. -- Function: void gal_type_min (uint8_t ‘type’, void ‘*in’) Put the minimum possible value of ‘type’ in the space pointed to by ‘in’. Since the value can have any type, this function doesn’t return anything, it assumes the space for the given type is available to ‘in’ and writes the value there. Here is one example int32_t min; gal_type_min(GAL_TYPE_INT32, &min); Note: Do not use the minimum value for a blank value of a general (initially unknown) type, please use the constants/functions provided in *note Library blank values:: for the definition and usage of blank values. -- Function: void gal_type_max (uint8_t ‘type’, void ‘*in’) Put the maximum possible value of ‘type’ in the space pointed to by ‘in’. Since the value can have any type, this function doesn’t return anything, it assumes the space for the given type is available to ‘in’ and writes the value there. Here is one example uint16_t max; gal_type_max(GAL_TYPE_INT16, &max); Note: Do not use the maximum value for a blank value of a general (initially unknown) type, please use the constants/functions provided in *note Library blank values:: for the definition and usage of blank values. -- Function: int gal_type_is_list (uint8_t ‘type’) Return 1 if the type is a linked list and zero otherwise. -- Function: int gal_type_out (int ‘first_type’, int ‘second_type’) Return the larger of the two given types which can be used for the type of the output of an operation involving the two input types. -- Function: char * gal_type_bit_string (void ‘*in’, size_t ‘size’) Return the bit-string in the ‘size’ bytes that ‘in’ points to. The string is dynamically allocated and must be freed afterwards. You can use it to inspect the bits within one region of memory. Here is one short example: int32_t a=2017; char *bitstr=gal_type_bit_string(&a, 4); printf("%d: %s (%X)\n", a, bitstr, a); free(bitstr); which will produce: 2017: 11100001000001110000000000000000 (7E1) As the example above shows, the bit-string is not the most efficient way to inspect bits. If you are familiar with hexadecimal notation, it is much more compact, see . You can use ‘printf’’s ‘%x’ or ‘%X’ to print integers in hexadecimal format. -- Function: char * gal_type_to_string (void ‘*ptr’, uint8_t ‘type’, int ‘quote_if_str_has_space’); Read the contents of the memory that ‘ptr’ points to (assuming it has type ‘type’ and print it into an allocated string which is returned. If the memory is a string of characters and ‘quote_if_str_has_space’ is non-zero, the output string will have double-quotes around it if it contains space characters. Also, note that in this case, ‘ptr’ must be a pointer to an array of characters (or ‘char **’), as in the example below (which will put ‘"sample string"’ into ‘out’): char *out, *string="sample string" out = gal_type_to_string(&string, GAL_TYPE_STRING, 1); -- Function: int gal_type_from_string (void ‘**out’, char ‘*string’, uint8_t ‘type’) Read a string as a given data type and put a the pointer to it in ‘*out’. When ‘*out!=NULL’, then it is assumed to be already allocated and the value will be simply put the memory. If ‘*out==NULL’, then space will be allocated for the given type and the string will be read into that type. Note that when we are dealing with a string type, ‘*out’ should be interpretted as ‘char **’ (one element in an array of pointers to different strings). In other words, ‘out’ should be ‘char ***’. This function can be used to fill in arrays of numbers from strings (in an already allocated data structure), or add nodes to a linked list (if the type is a list type). For an array, you have to pass the pointer to the ‘i’th element where you want the value to be stored, for example ‘&(array[i]’). If the string was successfully parsed to the requested type, this function will return a ‘0’ (zero), otherwise it will return ‘1’ (one). This output format will help you check the status of the conversion in a code like the example below: if( gal_type_from_string(&out, string, GAL_TYPE_FLOAT32) ) { fprintf(stderr, "%s couldn't be read as float32.\n", string); exit(EXIT_FAILURE); } -- Function: void * gal_type_string_to_number (char ‘*string’, uint8_t ‘*type’) Read ‘string’ into smallest type that can host the number, the allocated space for the number will be returned and the type of the number will be put into the memory that ‘type’ points to. If ‘string’ couldn’t be read as a number, this function will return ‘NULL’. For the ranges acceptable by each type see *note Numeric data types::. For integers it is clear, for floating point types, this function will count the number of significant digits and determine if the given string is single or double precision as described in that section. gnuastro-0.5/doc/gnuastro.info-20000644000175000017500000114500013217220435013564 00000000000000This is gnuastro.info, produced by makeinfo version 6.5 from gnuastro.texi. This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro’s library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Tables, Next: Tessellation, Prev: Numeric data types, Up: Common program behavior 4.5 Tables ========== “A table is a collection of related data held in a structured format within a database. It consists of columns, and rows.†(from Wikipedia). Each column in the table contains the values of one property and each row is a collection of properties (columns) for one target object. For example, let’s assume you have just ran MakeCatalog (see *note MakeCatalog::) on an image to measure some properties for the labeled regions (which might be detected galaxies for example) in the image. For each labeled region (detected galaxy), there will be a _row_ which groups its measured properties as _columns_, one column for each property. One such property can be the object’s magnitude, which is the sum of pixels with that label, or its center can be defined as the light-weighted average value of those pixels. Many such properties can be derived from the raw pixel values and their position, see *note Invoking astmkcatalog:: for a long list. As a summary, for each labeled region (or, galaxy) we have one _row_ and for each measured property we have one _column_. This high-level structure is usually the first step for higher-level analysis, for example finding the stellar mass or photometric redshift from magnitudes in multiple colors. Thus, tables are not just outputs of programs, in fact it is much more common for tables to be inputs of programs. For example, to make a mock galaxy image, you need to feed in the properties of each galaxy into *note MakeProfiles:: for it do the inverse of the process above and make a simulated image from a catalog, see *note Sufi simulates a detection::. In other cases, you can feed a table into *note Crop:: and it will crop out regions centered on the positions within the table, see *note Hubble visually checks and classifies his catalog::. So to end this relatively long introduction, tables play a very important role in astronomy, or generally all branches of data analysis. In *note Recognized table formats:: the currently recognized table formats in Gnuastro are discussed. You can use any of these tables as input or ask for them to be built as output. The most common type of table format is a simple plain text file with each row on one line and columns separated by white space characters, this format is easy to read/write by eye/hand. To give it the full functionality of more specific table types like the FITS tables, Gnuastro has a special convention which you can use to give each column a name, type, unit, and comments, while still being readable by other plain text table readers. This convention is described in *note Gnuastro text table format::. When tables are input to a program, the program reading it needs to know which column(s) it should use for its desired purposes. Gnuastro’s programs all follow a similar convention, on the way you can select columns in a table. They are thoroughly discussed in *note Selecting table columns::. * Menu: * Recognized table formats:: Table formats that are recognized in Gnuastro. * Gnuastro text table format:: Gnuastro’s convention plain text tables. * Selecting table columns:: Identify/select certain columns from a table  File: gnuastro.info, Node: Recognized table formats, Next: Gnuastro text table format, Prev: Tables, Up: Tables 4.5.1 Recognized table formats ------------------------------ The list of table formats that Gnuastro can currently read from and write to are described below. Each has their own advantage and disadvantages, so a short review of the format is also provided to help you make the best choice based on how you want to define your input tables or later use your output tables. Plain text table This is the most basic and simplest way to create, view, or edit the table by hand on a text editor. The other formats described below are less eye-friendly and have a more formal structure (for easier computer readability). It is fully described in *note Gnuastro text table format::. FITS ASCII tables The FITS ASCII table extension is fully in ASCII encoding and thus easily readable on any text editor (assuming it is the only extension in the FITS file). If the FITS file also contains binary extensions (for example an image or binary table extensions), then there will be many hard to print characters. The FITS ASCII format doesn’t have new line characters to separate rows. In the FITS ASCII table standard, each row is defined as a fixed number of characters (value to the ‘NAXIS1’ keyword), so to visually inspect it properly, you would have to adjust your text editor’s width to this value. All columns start at given character positions and have a fixed width (number of characters). Numbers in a FITS ASCII table are printed into ASCII format, they are not in binary (that the CPU uses). Hence, they can take a larger space in memory, loose their precision, and take longer to read into memory. If you are dealing with integer type columns (see *note Numeric data types::), another issue with FITS ASCII tables is that the type information for the column will be lost (there is only one integer type in FITS ASCII tables). One problem with the binary format on the other hand is that it isn’t portable (different CPUs/compilers) have different standards for translating the zeros and ones. But since ASCII characters are defined on a byte and are well recognized, they are better for portability on those various systems. Gnuastro’s plain text table format described below is much more portable and easier to read/write/interpret by humans manually. Generally, as the name implies, this format is useful for when your table mainly contains ASCII columns (for example file names, or descriptions). They can be useful when you need to include columns with structured ASCII information along with other extensions in one FITS file. In such cases, you can also consider header keywords (see *note Fits::). FITS binary tables The FITS binary table is the FITS standard’s solution to the issues discussed with keeping numbers in ASCII format as described under the FITS ASCII table title above. Only columns defined as a string type (a string of ASCII characters) are readable in a text editor. The portability problem with binary formats discussed above is mostly solved thanks to the portability of CFITSIO (see *note CFITSIO::) and the very long history of the FITS format which has been widely used since the 1970s. In the case of most numbers, storing them in binary format is more memory efficient than ASCII format. For example, to store ‘-25.72034’ in ASCII format, you need 9 bytes/characters. But if you keep this same number (to the approximate precision possible) as a 4-byte (32-bit) floating point number, you can keep/transmit it with less than half the amount of memory. When catalogs contain thousands/millions of rows in tens/hundreds of columns, this can lead to significant improvements in memory/band-width usage. Moreover, since the CPU does its operations in the binary formats, reading the table in and writing it out is also much faster than an ASCII table. When you are dealing with integer numbers, the compression ratio can be even better, for example if you know all of the values in a column are positive and less than ‘255’, you can use the ‘unsigned char’ type which only takes one byte! If they are between ‘-128’ and ‘127’, then you can use the (signed) ‘char’ type. So if you are thoughtful about the limits of your integer columns, you can greatly reduce the size of your file and also the speed at which it is read/written. This can be very useful when sharing your results with collaborators or publishing them. To decrease the file size even more you can name your output as ending in ‘.fits.gz’ so it is also compressed after creation. Just note that compression/decompressing is CPU intensive and can slow down the writing/reading of the file. Fortunately the FITS Binary table format also accepts ASCII strings as column types (along with the various numerical types). So your dataset can also contain non-numerical columns. * Menu: * Gnuastro text table format:: Reading plain text tables  File: gnuastro.info, Node: Gnuastro text table format, Next: Selecting table columns, Prev: Recognized table formats, Up: Tables 4.5.2 Gnuastro text table format -------------------------------- Plain text files are the most generic, portable, and easiest way to (manually) create, (visually) inspect, or (manually) edit a table. In this format, the ending of a row is defined by the new-line character (a line on a text editor). So when you view it on a text editor, every row will occupy one line. The delimiters (or characters separating the columns) are white space characters (space, horizontal tab, vertical tab) and a comma (<,>). The only further requirement is that all rows/lines must have the same number of columns. The columns don’t have to be exactly under each other and the rows can be arbitrarily long with different lengths. For example the following contents in a file would be interpreted as a table with 4 columns and 2 rows, with each element interpreted as a ‘double’ type (see *note Numeric data types::). 1 2.234948 128 39.8923e8 2 , 4.454 792 72.98348e7 However, the example above has no other information about the columns (it is just raw data, with no meta-data). To use this table, you have to remember what the numbers in each column represent. Also, when you want to select columns, you have to count their position within the table. This can become frustrating and prone to bad errors (getting the columns wrong) especially as the number of columns increase. It is also bad for sending to a colleague, because they will find it hard to remember/use the columns properly. To solve these problems in Gnuastro’s programs/libraries you aren’t limited to using the column’s number, see *note Selecting table columns::. If the columns have names, units, or comments you can also select your columns based on searches/matches in these fields, for example see *note Table::. Also, in this manner, you can’t guide the program reading the table on how to read the numbers. As an example, the first and third columns above can be read as integer types: the first column might be an ID and the third can be the number of pixels an object occupies in an image. So there is no need to read these to columns as a ‘double’ type (which takes more memory, and is slower). In the bare-minimum example above, you also can’t use strings of characters, for example the names of filters, or some other identifier that includes non-numerical characters. In the absence of any information, only numbers can be read robustly. Assuming we read columns with non-numerical characters as string, there would still be the problem that the strings might contain space (or any delimiter) character for some rows. So, each ‘word’ in the string will be interpreted as a column and the program will abort with an error that the rows don’t have the same number of columns. To correct for these limitations, Gnuastro defines the following convention for storing the table meta-data along with the raw data in one plain text file. The format is primarily designed for ease of reading/writing by eye/fingers, but is also structured enough to be read by a program. When the first non-white character in a line is <#>, or there are no non-white characters in it, then the line will not be considered as a row of data in the table (this is a pretty standard convention in many programs, and higher level languages). In the former case, the line is interpreted as a _comment_. If the comment line starts with ‘‘# Column N:’’, then it is assumed to contain information about column ‘N’ (a number, counting from 1). Comment lines that don’t start with this pattern are ignored and you can use them to include any further information you want to store with the table in the text file. A column information comment is assumed to have the following format: # Column N: NAME [UNIT, TYPE, BLANK] COMMENT Any sequence of characters between ‘<:>’ and ‘<[>’ will be interpreted as the column name (so it can contain anything except the ‘<[>’ character). Anything between the ‘<]>’ and the end of the line is defined as a comment. Within the brackets, anything before the first ‘<,>’ is the units (physical units, for example km/s, or erg/s), anything before the second ‘<,>’ is the short type identifier (see below, and *note Numeric data types::). Finally (still within the brackets), any non-white characters after the second ‘<,>’ are interpreted as the blank value for that column (see *note Blank pixels::). Note that blank values will be stored in the same type as the column, not as a string(1). When a formatting problem occurs (for example you have specified the wrong type code, see below), or the the column was already given meta-data in a previous comment, or the column number is larger than the actual number of columns in the table (the non-commented or empty lines), then the comment information line will be ignored. When a comment information line can be used, the leading and trailing white space characters will be stripped from all of the elements. For example in this line: # Column 5: column name [km/s, f32,-99] Redshift as speed The ‘NAME’ field will be ‘‘column name’’ and the ‘TYPE’ field will be ‘‘f32’’. Note how all the white space characters before and after strings are not used, but those in the middle remained. Also, white space characters aren’t mandatory. Hence, in the example above, the ‘BLANK’ field will be given the value of ‘‘-99’’. Except for the column number (‘N’), the rest of the fields are optional. Also, the column information comments don’t have to be in order. In other words, the information for column $N+m$ ($m>0$) can be given in a line before column $N$. Also, you don’t have to specify information for all columns. Those columns that don’t have this information will be interpreted with the default settings (like the case above: values are double precision floating point, and the column has no name, unit, or comment). So these lines are all acceptable for any table (the first one, with nothing but the column number is redundant): # Column 5: # Column 1: ID [,i] The Clump ID. # Column 3: mag_f160w [AB mag, f] Magnitude from the F160W filter The data type of the column should be specified with one of the following values: • For a numeric column, you can use any of the numeric types (and their recognized identifiers) described in *note Numeric data types::. • ‘‘strN’’: for strings. The ‘N’ value identifies the length of the string (how many characters it has). The start of the string on each row is the first non-delimiter character of the column that has the string type. The next ‘N’ characters will be interpreted as a string and all leading and trailing white space will be removed. If the next column’s characters, are closer than ‘N’ characters to the start of the string column in that line/row, they will be considered part of the string column. If there is a new-line character before the ending of the space given to the string column (in other words, the string column is the last column), then reading of the string will stop, even if the ‘N’ characters are not complete yet. See ‘tests/table/table.txt’ for one example. Therefore, the only time you have to pay attention to the positioning and spaces given to the string column is when it is not the last column in the table. The only limitation in this format is that trailing and leading white space characters will be removed from the columns that are read. In most cases, this is the desired behavior, but if trailing and leading white-spaces are critically important to your analysis, define your own starting and ending characters and remove them after the table has been read. For example in the sample table below, the two ‘<|>’ characters (which are arbitrary) will remain in the value of the second column and you can remove them manually later. If only one of the leading or trailing white spaces is important for your work, you can only use one of the ‘<|>’s. # Column 1: ID [label, uc] # Column 2: Notes [no unit, str50] 1 leading and trailing white space is ignored here 2.3442e10 2 | but they will be preserved here | 8.2964e11 Note that the FITS binary table standard does not define the ‘unsigned int’ and ‘unsigned long’ types, so if you want to convert your tables to FITS binary tables, use other types. Also, note that in the FITS ASCII table, there is only one integer type (‘long’). So if you convert a Gnuastro plain text table to a FITS ASCII table with the *note Table:: program, the type information for integers will be lost. Conversely if integer types are important for you, you have to manually set them when reading a FITS ASCII table (for example with the Table program when reading/converting into a file, or with the ‘gnuastro/table.h’ library functions when reading into memory). ---------- Footnotes ---------- (1) For floating point types, the ‘nan’, or ‘inf’ strings (both not case-sensitive) refer to IEEE NaN (not a number) and infinity values respectively and will be stored as a floating point, so they are acceptable.  File: gnuastro.info, Node: Selecting table columns, Prev: Gnuastro text table format, Up: Tables 4.5.3 Selecting table columns ----------------------------- At the lowest level, the only defining aspect of a column in a table is its number, or position. But selecting columns purely by number is not very convenient and, especially when the tables are large it can be very frustrating and prone to errors. Hence, table file formats (for example see *note Recognized table formats::) have ways to store additional information about the columns (meta-data). Some of the most common pieces of information about each column are its _name_, the _units_ of data in the it, and a _comment_ for longer/informal description of the column’s data. To facilitate research with Gnuastro, you can select columns by matching, or searching in these three fields, besides the low-level column number. To view the full list of information on the columns in the table, you can use the Table program (see *note Table::) with the command below (replace ‘table-file’ with the filename of your table, if its FITS, you might also need to specify the HDU/extension which contains the table): $ asttable --information table-file Gnuastro’s programs need the columns for different purposes, for example in Crop, you specify the columns containing the central coordinates of the crop centers with the ‘--coordcol’ option (see *note Crop options::). On the other hand, in MakeProfiles, to specify the column containing the profile position angles, you must use the ‘--pcol’ option (see *note MakeProfiles catalog::). Thus, there can be no unified common option name to select columns for all programs (different columns have different purposes). However, when the program expects a column for a specific context, the option names end in the ‘col’ suffix like the examples above. These options accept values in integer (column number), or string (metadata match/search) format. If the value can be parsed as a positive integer, it will be seen as the low-level column number. Note that column counting starts from 1, so if you ask for column 0, the respective program will abort with an error. When the value can’t be interpreted as an a integer number, it will be seen as a string of characters which will be used to match/search in the table’s meta-data. The meta-data field which the value will be compared with can be selected through the ‘--searchin’ option, see *note Input output options::. ‘--searchin’ can take three values: ‘name’, ‘unit’, ‘comment’. The matching will be done following this convention: • If the value is enclosed in two slashes (for example ‘-x/RA_/’, or ‘--coordcol=/RA_/’, see *note Crop options::), then it is assumed to be a regular expression with the same convention as GNU AWK. GNU AWK has a very well written chapter (https://www.gnu.org/software/gawk/manual/html_node/Regexp.html) describing regular expressions, so we we will not continue discussing them here. Regular expressions are a very powerful tool in matching text and useful in many contexts. We thus strongly encourage reviewing this chapter for greatly improving the quality of your work in many cases, not just for searching column meta-data in Gnuastro. • When the string isn’t enclosed between ‘’s, any column that exactly matches the given value in the given field will be selected. Note that in both cases, you can ignore the case of alphabetic characters with the ‘--ignorecase’ option, see *note Input output options::. Also, in both cases, multiple columns may be selected with one call to this function. In this case, the order of the selected columns (with one call) will be the same order as they appear in the table.  File: gnuastro.info, Node: Tessellation, Next: Getting help, Prev: Tables, Up: Common program behavior 4.6 Tessellation ================ It is sometimes necessary to classify the elements in a dataset (for example pixels in an image) into a grid of individual, non-overlapping tiles. For example when background sky gradients are present in an image, you can define a tile grid over the image. When the tile sizes are set properly, the background’s variation over each tile will be negligible, allowing you to measure (and subtract) it. In other cases (for example spatial domain convolution in Gnuastro, see *note Convolve::), it might simply be for speed of processing: each tile can be processed independently on a separate CPU thread. In the arts and mathematics, this process is formally known as tessellation (https://en.wikipedia.org/wiki/Tessellation). The size of the regular tiles (in units of data-elements, or pixels in an image) can be defined with the ‘--tilesize’ option. It takes multiple numbers (separated by a comma) which will be the length along the respective dimension (in FORTRAN/FITS dimension order). Divisions are also acceptable, but must result in an integer. For example ‘--tilesize=30,40’ can be used for an image (a 2D dataset). The regular tile size along the first FITS axis (horizontal when viewed in SAO ds9) will be 30 pixels and along the second it will be 40 pixels. Ideally, ‘--tilesize’ should be selected such that all tiles in the image have exactly the same size. In other words, that the dataset length in each dimension is divisible by the tile size in that dimension. However, this is not always possible: the dataset can be any size and every pixel in it is valuable. In such cases, Gnuastro will look at the significance of the remainder length, if it is not significant (for example one or two pixels), then it will just increase the size of the first tile in the respective dimension and allow the rest of the tiles to have the required size. When the remainder is significant (for example one pixel less than the size along that dimension), the remainder will be added to one regular tile’s size and the large tile will be cut in half and put in the two ends of the grid/tessellation. In this way, all the tiles in the central regions of the dataset will have the regular tile sizes and the tiles on the edge will be slightly larger/smaller depending on the remainder significance. The fraction which defines the remainder significance along all dimensions can be set through ‘--remainderfrac’. The best tile size is directly related to the spatial properties of the property you want to study (for example, gradient on the image). In practice we assume that the gradient is not present over each tile. So if there is a strong gradient (for example in long wavelength ground based images) or the image is of a crowded area where there isn’t too much blank area, you have to choose a smaller tile size. A larger mesh will give more pixels and and so the scatter in the results will be less (better statistics). For raw image processing, a single tessellation/grid is not sufficient. Raw images are the unprocessed outputs of the camera detectors. Modern detectors usually have multiple readout channels each with its own amplifier. For example the Hubble Space Telescope Advanced Camera for Surveys (ACS) has four amplifiers over its full detector area dividing the square field of view to four smaller squares. Ground based image detectors are not exempt, for example each CCD of Subaru Telescope’s Hyper Suprime-Cam camera (which has 104 CCDs) has four amplifiers, but they have the same height of the CCD and divide the width by four parts. The bias current on each amplifier is different, and initial bias subtraction is not perfect. So even after subtracting the measured bias current, you can usually still identify the boundaries of different amplifiers by eye. See Figure 11(a) in Akhlaghi and Ichikawa (2015) for an example. This results in the final reduced data to have non-uniform amplifier-shaped regions with higher or lower background flux values. Such systematic biases will then propagate to all subsequent measurements we do on the data (for example photometry and subsequent stellar mass and star formation rate measurements in the case of galaxies). Therefore an accurate analysis requires a two layer tessellation: the top layer contains larger tiles, each covering one amplifier channel. For clarity we’ll call these larger tiles “channelsâ€. The number of channels along each dimension is defined through the ‘--numchannels’. Each channel is then covered by its own individual smaller tessellation (with tile sizes determined by the ‘--tilesize’ option). This will allow independent analysis of two adjacent pixels from different channels if necessary. If the image is processed or the detector only has one amplifier, you can set the number of channels in both dimension to 1. The final tessellation can be inspected on the image with the ‘--checktiles’ option that is available to all programs which use tessellation for localized operations. When this option is called, a FITS file with a ‘_tiled.fits’ suffix will be created along with the outputs, see *note Automatic output::. Each pixel in this image has the number of the tile that covers it. If the number of channels in any dimension are larger than unity, you will notice that the tile IDs are defined such that the first channels is covered first, then the second and so on. For the full list of processing-related common options (including tessellation options), please see *note Processing options::.  File: gnuastro.info, Node: Getting help, Next: Automatic output, Prev: Tessellation, Up: Common program behavior 4.7 Getting help ================ Probably the first time you read this book, it is either in the PDF or HTML formats. These two formats are very convenient for when you are not actually working, but when you are only reading. Later on, when you start to use the programs and you are deep in the middle of your work, some of the details will inevitably be forgotten. Going to find the PDF file (printed or digital) or the HTML webpage is a major distraction. GNU software have a very unique set of tools for aiding your memory on the command-line, where you are working, depending how much of it you need to remember. In the past, such command-line help was known as “online†help, because they were literally provided to you ‘on’ the command ‘line’. However, nowadays the word “online†refers to something on the internet, so that term will not be used. With this type of help, you can resume your exciting research without taking your hands off the keyboard. Another major advantage of such command-line based help routines is that they are installed with the software in your computer, therefore they are always in sync with the executable you are actually running. Three of them are actually part of the executable. You don’t have to worry about the version of the book or program. If you rely on external help (a PDF in your personal print or digital archive or HTML from the official webpage) you have to check to see if their versions fit with your installed program. If you only need to remember the short or long names of the options, ‘--usage’ is advised. If it is what the options do, then ‘--help’ is a great tool. Man pages are also provided for those who are use to this older system of documentation. This full book is also available to you on the command-line in Info format. If none of these seems to resolve the problems, there is a mailing list which enables you to get in touch with experienced Gnuastro users. In the subsections below each of these methods are reviewed. * Menu: * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from –help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users.  File: gnuastro.info, Node: --usage, Next: --help, Prev: Getting help, Up: Getting help 4.7.1 ‘--usage’ --------------- If you give this option, the program will not run. It will only print a very concise message showing the options and arguments. Everything within square brackets (‘[]’) is optional. For example here are the first and last two lines of Crop’s ‘--usage’ is shown: $ astcrop --usage Usage: astcrop [-Do?IPqSVW] [-d INT] [-h INT] [-r INT] [-w INT] [-x INT] [-y INT] [-c INT] [-p STR] [-N INT] [--deccol=INT] .... [--setusrconf] [--usage] [--version] [--wcsmode] [ASCIIcatalog] FITSimage(s).fits There are no explanations on the options, just their short and long names shown separately. After the program name, the short format of all the options that don’t require a value (on/off options) is displayed. Those that do require a value then follow in separate brackets, each displaying the format of the input they want, see *note Options::. Since all options are optional, they are shown in square brackets, but arguments can also be optional. For example in this example, a catalog name is optional and is only required in some modes. This is a standard method of displaying optional arguments for all GNU software.  File: gnuastro.info, Node: --help, Next: Man pages, Prev: --usage, Up: Getting help 4.7.2 ‘--help’ -------------- If the command-line includes this option, the program will not be run. It will print a complete list of all available options along with a short explanation. The options are also grouped by their context. Within each context, the options are sorted alphabetically. Since the options are shown in detail afterwards, the first line of the ‘--help’ output shows the arguments and if they are optional or not, similar to *note --usage::. In the ‘--help’ output of all programs in Gnuastro, the options for each program are classified based on context. The first two contexts are always options to do with the input and output respectively. For example input image extensions or supplementary input files for the inputs. The last class of options is also fixed in all of Gnuastro, it shows operating mode options. Most of these options are already explained in *note Operating mode options::. The help message will sometimes be longer than the vertical size of your terminal. If you are using a graphical user interface terminal emulator, you can scroll the terminal with your mouse, but we promised no mice distractions! So here are some suggestions: • to scroll up and to scroll down. For most help output this should be enough. The problem is that it is limited by the number of lines that your terminal keeps in memory and that you can’t scroll by lines, only by whole screens. • Pipe to ‘less’. A pipe is a form of shell re-direction. The ‘less’ tool in Unix-like systems was made exactly for such outputs of any length. You can pipe (‘|’) the output of any program that is longer than the screen to it and then you can scroll through (up and down) with its many tools. For example: $ astnoisechisel --help | less Once you have gone through the text, you can quit ‘less’ by pressing the key. • Redirect to a file. This is a less convenient way, because you will then have to open the file in a text editor! You can do this with the shell redirection tool (‘>’): $ astnoisechisel --help > filename.txt In case you have a special keyword you are looking for in the help, you don’t have to go through the full list. GNU Grep is made for this job. For example if you only want the list of options whose ‘--help’ output contains the word “axis†in Crop, you can run the following command: $ astcrop --help | grep axis If the output of this option does not fit nicely within the confines of your terminal, GNU does enable you to customize its output through the environment variable ‘ARGP_HELP_FMT’, you can set various parameters which specify the formatting of the help messages. For example if your terminals are wider than 70 spaces (say 100) and you feel there is too much empty space between the long options and the short explanation, you can change these formats by giving values to this environment variable before running the program with the ‘--help’ output. You can define this environment variable in this manner: $ export ARGP_HELP_FMT=rmargin=100,opt-doc-col=20 This will affect all GNU programs using GNU C library’s ‘argp.h’ facilities as long as the environment variable is in memory. You can see the full list of these formatting parameters in the “Argp User Customization†part of the GNU C library manual. If you are more comfortable to read the ‘--help’ outputs of all GNU software in your customized format, you can add your customizations (similar to the line above, without the ‘$’ sign) to your ‘~/.bashrc’ file. This is a standard option for all GNU software.  File: gnuastro.info, Node: Man pages, Next: Info, Prev: --help, Up: Getting help 4.7.3 Man pages --------------- Man pages were the Unix method of providing command-line documentation to a program. With GNU Info, see *note Info:: the usage of this method of documentation is highly discouraged. This is because Info provides a much more easier to navigate and read environment. However, some operating systems require a man page for packages that are installed and some people are still used to this method of command line help. So the programs in Gnuastro also have Man pages which are automatically generated from the outputs of ‘--version’ and ‘--help’ using the GNU help2man program. So if you run $ man programname You will be provided with a man page listing the options in the standard manner.  File: gnuastro.info, Node: Info, Next: help-gnuastro mailing list, Prev: Man pages, Up: Getting help 4.7.4 Info ---------- Info is the standard documentation format for all GNU software. It is a very useful command-line document viewing format, fully equipped with links between the various pages and menus and search capabilities. As explained before, the best thing about it is that it is available for you the moment you need to refresh your memory on any command-line tool in the middle of your work without having to take your hands off the keyboard. This complete book is available in Info format and can be accessed from anywhere on the command-line. To open the Info format of any installed programs or library on your system which has an Info format book, you can simply run the command below (change ‘executablename’ to the executable name of the program or library): $ info executablename In case you are not already familiar with it, run ‘$ info info’. It does a fantastic job in explaining all its capabilities its self. It is very short and you will become sufficiently fluent in about half an hour. Since all GNU software documentation is also provided in Info, your whole GNU/Linux life will significantly improve. Once you’ve become an efficient navigator in Info, you can go to any part of this book or any other GNU software or library manual, no matter how long it is, in a matter of seconds. It also blends nicely with GNU Emacs (a text editor) and you can search manuals while you are writing your document or programs without taking your hands off the keyboard, this is most useful for libraries like the GNU C library. To be able to access all the Info manuals installed in your GNU/Linux within Emacs, type . To see this whole book from the beginning in Info, you can run $ info gnuastro If you run Info with the particular program executable name, for example ‘astcrop’ or ‘astnoisechisel’: $ info astprogramname you will be taken to the section titled “Invoking ProgramName†which explains the inputs and outputs along with the command-line options for that program. Finally, if you run Info with the official program name, for example Crop or NoiseChisel: $ info ProgramName you will be taken to the top section which introduces the program. Note that in all cases, Info is not case sensitive.  File: gnuastro.info, Node: help-gnuastro mailing list, Prev: Info, Up: Getting help 4.7.5 help-gnuastro mailing list -------------------------------- Gnuastro maintains the help-gnuastro mailing list for users to ask any questions related to Gnuastro. The experienced Gnuastro users and some of its developers are subscribed to this mailing list and your email will be sent to them immediately. However, when contacting this mailing list please have in mind that they are possibly very busy and might not be able to answer immediately. To ask a question from this mailing list, send a mail to ‘help-gnuastro@gnu.org’. Anyone can view the mailing list archives at . It is best that before sending a mail, you search the archives to see if anyone has asked a question similar to yours. If you want to make a suggestion or report a bug, please don’t send a mail to this mailing list. We have other mailing lists and tools for those purposes, see *note Report a bug:: or *note Suggest new feature::.  File: gnuastro.info, Node: Automatic output, Next: Output headers, Prev: Getting help, Up: Common program behavior 4.8 Automatic output ==================== All the programs in Gnuastro are designed such that specifying an output file or directory (based on the program context) is optional. The outputs of most programs are automatically found based on the input and what the program does. For example when you are converting a FITS image named ‘FITSimage.fits’ to a JPEG image, the JPEG image will be saved in ‘FITSimage.jpg’. Another very important part of the automatic output generation is that all the directory information of the input file name is stripped off of it. This feature can be disabled with the ‘--keepinputdir’ option, see *note Common options::. It is the default because astronomical data are usually very large and organized specially with special file names. In some cases, the user might not have write permissions in those directories. In fact, even if the data is stored on your own computer, it is advised to only grant write permissions to the super user or root. This way, you won’t accidentally delete or modify your valuable data! Let’s assume that we are working on a report and want to process the FITS images from two projects (ABC and DEF), which are stored in the sub-directories named ‘ABCproject/’ and ‘DEFproject/’ of our top data directory (‘/mnt/data’). The following shell commands show how one image from the former is first converted to a JPEG image through ConvertType and then the objects from an image in the latter project are detected using NoiseChisel. The text after the ‘#’ sign are comments (not typed!). $ pwd # Current location /home/usrname/research/report $ ls # List directory contents ABC01.jpg $ ls /mnt/data/ABCproject # Archive 1 ABC01.fits ABC02.fits ABC03.fits $ ls /mnt/data/DEFproject # Archive 2 DEF01.fits DEF02.fits DEF03.fits $ astconvertt /mnt/data/ABCproject/ABC02.fits --output=jpg # Prog 1 $ ls ABC01.jpg ABC02.jpg $ astnoisechisel /mnt/data/DEFproject/DEF01.fits # Prog 2 $ ls ABC01.jpg ABC02.jpg DEF01_labeled.fits  File: gnuastro.info, Node: Output headers, Prev: Automatic output, Up: Common program behavior 4.9 Output headers ================== The output FITS files created by Gnuastro’s programs have some or all of the following standard keywords to keep the basic date and version information of Gnuastro, its dependencies and the pipeline that is using Gnuastro. ‘DATE’ The creation time of the FITS file. This date is written directly by CFITSIO and is in UT format. ‘COMMIT’ Git’s commit description from the running directory of Gnuastro’s programs. If the running directory is not version controlled or ‘libgit2’ isn’t installed (see *note Optional dependencies::) then this keyword will not be present. The printed value is equivalent to the output of the following command: git describe --dirty --always If the running directory contains non-committed work, then the stored value will have a ‘‘-dirty’’ suffix. This can be very helpful to let you know that the data is not ready to be shared with collaborators or submitted to a journal. You should only share results that are produced after all your work is committed (safely stored in the version controlled history and thus reproducible). At first sight, version control appears to be mainly a tool for software developers. However progress in a scientific research is almost identical to progress in software development: first you have a rough idea that starts with handful of easy steps. But as the first results appear to be promising, you will have to extend, or generalize, it to make it more robust and work in all the situations your research covers, not just your first test samples. Slowly you will find wrong assumptions or bad implementations that need to be fixed (‘bugs’ in software development parlance). Finally, when you submit the research to your collaborators or a journal, many comments and suggestions will come in, and you have to address them. Software developers have created version control systems precisely for this kind of activity. Each significant moment in the project’s history is called a “commitâ€, see *note Version controlled source::. A snapshot of the project in each “commit†is safely stored away, so you can revert back to it at a later time, or check changes/progress. This way, you can be sure that your work is reproducible and track the progress and history. With version control, experimentation in the project’s analysis is greatly facilitated, since you can easily revert back if a brainstorm test procedure fails. One important feature of version control is that the research result (FITS image, table, report or paper) can be stamped with the unique commit information that produced it. This information will enable you to exactly reproduce that same result later, even if you have made changes/progress. For one example of a research paper’s reproduction pipeline, please see the reproduction pipeline (https://gitlab.com/makhlaghi/NoiseChisel-paper) of the paper (https://arxiv.org/abs/1505.01664) describing *note NoiseChisel::. ‘CFITSIO’ The version of CFITSIO used (see *note CFITSIO::). ‘WCSLIB’ The version of WCSLIB used (see *note WCSLIB::). Note that older versions of WCSLIB do not report the version internally. So this is only available if you are using more recent WCSLIB versions. ‘GSL’ The version of GNU Scientific Library that was used, see *note GNU Scientific Library::. ‘GNUASTRO’ The version of Gnuastro used (see *note Version numbering::). Here is one example of the last few lines of an example output. / Versions and date DATE = '...' / file creation date COMMIT = 'v0-8-g547f6eb' / Commit description in running dir. CFITSIO = '3.41 ' / CFITSIO version. WCSLIB = '5.16 ' / WCSLIB version. GSL = '2.3 ' / GNU Scientific Library version. GNUASTRO= '0.3' / GNU Astronomy Utilities version. END  File: gnuastro.info, Node: Data containers, Next: Data manipulation, Prev: Common program behavior, Up: Top 5 Data containers ***************** The most low-level and basic property of a dataset is how it is stored. To process, archive and transmit the data, you need a container to store it first. From the start of the computer age, different formats have been defined to store data, optimized for particular applications. One format/container can never be useful for all applications: the storage defines the application and vice-versa. In astronomy, the Flexible Image Transport System (FITS) standard has become the most common format of data storage and transmission. It has many useful features, for example multiple sub-containers (also known as extensions or header data units, HDUs) within one file, or support for tables as well as images. Each HDU can store an independent dataset and its corresponding meta-data. Therefore, Gnuastro has one program (see *note Fits::) specifically designed to manipulate FITS HDUs and the meta-data (header keywords) in each HDU. Your astronomical research does not just involve data analysis (where the FITS format is very useful). For example you want to demonstrate your raw and processed FITS images or spectra as figures within slides, reports, or papers. The FITS format is not defined for such applications. Thus, Gnuastro also comes with the ConvertType program (see *note ConvertType::) which can be used to convert a FITS image to and from (where possible) other formats like plain text and JPEG (which allow two way conversion), along with EPS and PDF (which can only be created from FITS, not the other way round). Finally, the FITS format is not just for images, it can also store tables. Binary tables in particular can be very efficient in storing catalogs that have more than a few tens of columns and rows. However, unlike images (where all elements/pixels have one data type), tables contain multiple columns and each column can have different properties: independent data types (see *note Numeric data types::) and meta-data. In practice, each column can be viewed as a separate container that is grouped with others in the table. The only shared property of the columns in a table is thus the number of elements they contain. To allow easy inspection/manipulation of table columns, Gnuastro has the Table program (see *note Table::). It can be used to select certain table columns in a FITS table and see them as a human readable output on the command-line, or to save them into another plain text or FITS table. * Menu: * Fits:: View and manipulate extensions and keywords. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text.  File: gnuastro.info, Node: Fits, Next: ConvertType, Prev: Data containers, Up: Data containers 5.1 Fits ======== The “Flexible Image Transport Systemâ€, or FITS, is by far the most common data container format in astronomy. Although the full name of the standard invokes the idea that it is only for images, it also contains very complete and robust features for tables. It started off in the 1970s and was formally published as a standard in 1981, it was adopted by the International Astronomical Union (IAU) in 1982 and an IAU working group to maintain its future was defined in 1988. The FITS 2.0 and 3.0 standards were approved in 2000 and 2008 respectively, and the 4.0 draft has also been released recently, please see the FITS standard document webpage (https://fits.gsfc.nasa.gov/fits_standard.html) for the full text of all versions. Also see the FITS 3.0 standard paper (https://doi.org/10.1051/0004-6361/201015362) for a nice introduction and history along with the full standard. Other formats, for example a JPEG image, only have one image/dataset per file, however one great advantage of the FITS standard is that it allows you to keep multiple datasets (images or tables along with their meta-data) in one file. Each data + metadata is known as an extension, or more formally a header data unit or HDU, in the FITS standard. In theory the HDUs can be completely independent: you can have multiple images of different dimensions/sizes or tables as separate extensions in one file. However, while the standard doesn’t impose any constraints on the relation between the datasets, it is strongly encouraged to group data that are contextually related with each other in one file. For example an image and the table/catalog of objects and their measured properties in that image. Another example can be multiple images of one patch of sky in different colors (filters). As discussed above, the extensions in a FITS file can be completely independent. To keep some information (meta-data) about the group of extensions in the FITS file, the community has adopted the following convention: put no data in the first extension, so it is just meta-data. This extension can thus be used to store Meta-data regarding the whole file (grouping of extensions). Subsequent extensions may contain data along with their own separate meta-data. All of Gnuastro’s programs also follow this convention: the main dataset (image or table) is in the second extension. See the example list of extension properties in *note Invoking astfits::. The meta-data contain information about the data, for example which region of the sky an image corresponds to, the units of the data, what telescope, camera, and filter the data were taken with, the software that produced it, or it observation or processing date. Hence without the meta-data, the raw dataset is practically just a collection of numbers and really hard to understand, or connect with the real world (other datasets). It is thus strongly encouraged to supplement your data (at any level of processing) with as much meta-data about your processing/science as possible. The meta-data of a FITS file is in ASCII format, which can be easily viewed or edited with a text editor or on the command-line. Each meta-data element (known as a keyword generally) is composed of a name, value, units and comments (the last two are optional). For example below you can see three FITS meta-data keywords for specifying the world coordinate system (WCS, or its location in the sky) of a dataset: LATPOLE = -27.805089 / [deg] Native latitude of celestial pole RADESYS = 'FK5' / Equatorial coordinate system EQUINOX = 2000.0 / [yr] Equinox of equatorial coordinates However, there are some limitations which discourage viewing/editing the keywords with text editors. For example there is a fixed length of 80 characters for each keyword (its name, value, units and comments) and there are no new-line characters, so on a text editor all the keywords are seen in one line. Also, the meta-data keywords are immediately followed by the data which are commonly in binary format and will show up as strange looking characters on a text editor, and significantly slowing down the processor. Gnuastro’s Fits program was designed to allow easy manipulation of FITS extensions and meta-data keywords on the command-line while conforming fully with the FITS standard. For example you can copy or cut (copy and remove) HDUs/extensions from one FITS file to another, or completely delete them. It also has features to delete, add, or edit meta-data keywords within one HDU. * Menu: * Invoking astfits:: Arguments and options to Header.  File: gnuastro.info, Node: Invoking astfits, Prev: Fits, Up: Fits 5.1.1 Invoking Fits ------------------- Fits can print or manipulate the FITS file HDUs (extensions), meta-data keywords in a given HDU. The executable name is ‘astfits’ with the following general template $ astfits [OPTION...] ASTRdata One line examples: ## View general information about every extension: $ astfits image.fits ## Print the header keywords in the second HDU (counting from 0): $ astfits image.fits -h1 ## Only print header keywords that contain `NAXIS': $ astfits image.fits -h1 | grep NAXIS ## Only print the WCS standard PC matrix elements $ astfits image.fits -h1 | grep 'PC._.' ## Copy a HDU from input.fits to out.fits: $ astfits input.fits --copy=hdu-name --output=out.fits ## Update the OLDKEY keyword value to 153.034: $ astfits --update=OLDKEY,153.034,"Old keyword comment" ## Delete one COMMENT keyword and add a new one: $ astfits --delete=COMMENT --comment="Anything you like ;-)." ## Write two new keywords with different values and comments: $ astfits --write=MYKEY1,20.00,"An example keyword" --write=MYKEY2,fd When no action is requested (and only a file name is given), Fits will print a list of information about the extension(s) in the file. This information includes the HDU number, HDU name (‘EXTNAME’ keyword), type of data (see *note Numeric data types::, and the number of data elements it contains (size along each dimension for images and table rows and columns). You can use this to get a general idea of the contents of the FITS file and what HDU to use for further processing, either with the Fits program or any other Gnuastro program. Here is one example of information about a FITS file with four extensions: the first extension has no data, it is a purely meta-data HDU (commonly used to keep meta-data about the whole file, or grouping of extensions, see *note Fits::). The second extension is an image with name ‘IMAGE’ and single precision floating point type (‘float32’, see *note Numeric data types::), it has 4287 pixels along its first (horizontal) axis and 4286 pixels along its second (vertical) axis. The third extension is also an image with name ‘MASK’. It is in 2-byte integer format (‘int16’) which is commonly used to keep information about pixels (for example to identify which ones were saturated, or which ones had cosmic rays and so on), note how it has the same size as the ‘IMAGE’ extension. The third extension is a binary table called ‘CATALOG’ which has 12371 rows and 5 columns (it probably contains information about the sources in the image). GNU Astronomy Utilities X.X Run on Day Month DD HH:MM:SS YYYY ----- HDU (extension) information: `image.fits'. Column 1: Index (counting from 0). Column 2: Name (`EXTNAME' in FITS standard). Column 3: Image data type or `table' format (ASCII or binary). Column 4: Size of data in HDU. ----- 0 n/a uint8 0 1 IMAGE float32 4287x4286 2 MASK int16 4287x4286 3 CATALOG table_binary 12371x5 If a specific HDU is identified on the command-line with the ‘--hdu’ (or ‘-h’ option) and no operation requested, then the full list of header keywords in that HDU will be printed (as if the ‘--printallkeys’ was called, see below). It is important to remember that this only occurs when ‘--hdu’ is given on the command-line. The ‘--hdu’ value given in a configuration file will only be used when a specific operation on keywords requested. Therefore as described in the paragraphs above, when no explicit call to the ‘--hdu’ option is made on the command-line and no operation is requested (on the command-line or configuration files), the basic information of each HDU/extension is printed. The operating mode and input/output options to Fits are similar to the other programs and fully described in *note Common options::. The options particular to Fits can be divided into two groups: 1) those related to modifying HDUs or extensions (see *note HDU manipulation::), and 2) those related to viewing/modifying meta-data keywords (see *note Keyword manipulation::). These two classes of options cannot be called together in one run: you can either work on the extensions or meta-data keywords in any instance of Fits. * Menu: * HDU manipulation:: Manipulate HDUs within a FITS file. * Keyword manipulation:: Manipulate metadata keywords in a HDU  File: gnuastro.info, Node: HDU manipulation, Next: Keyword manipulation, Prev: Invoking astfits, Up: Invoking astfits 5.1.1.1 HDU manipulation ........................ Each header data unit, or HDU (also known as an extension), in a FITS file is an independent dataset (data + meta-data). Multiple HDUs can be stored in one FITS file, see *note Fits::. The HDU modifying options to the Fits program are listed below. These options may be called multiple times in one run. If so, the extensions will be copied from the input FITS file to the output FITS file in the given order (on the command-line and also in configuration files, see *note Configuration file precedence::). If the separate classes are called together in one run of Fits, then first ‘--copy’ is run (on all specified HDUs), followed by ‘--cut’ (again on all specified HDUs), and then ‘--remove’ (on all specified HDUs). The ‘--copy’ and ‘--cut’ options need an output FITS file (specified with the ‘--output’ option). If the output file exists, then the specified HDU will be copied following the last extension of the output file (the existing HDUs in it will be untouched). Thus, after Fits finishes, the copied HDU will be the last HDU of the output file. If no output file name is given, then automatic output will be used to store the HDUs given to this option (see *note Automatic output::). ‘-C STR’ ‘--copy=STR’ Copy the specified extension into the output file, see explanations above. ‘-k STR’ ‘--cut=STR’ Cut (copy to output, remove from input) the specified extension into the output file, see explanations above. ‘-R STR’ ‘--remove=STR’ Remove the specified HDU from the input file. From CFITSIO: “In the case of deleting the primary array (the first HDU in the file) then [it] will be replaced by a null primary array containing the minimum set of required keywords and no data.â€. So in practice, any existing data (array) and meta-data in the first extension will be removed, but the number of extensions in the file won’t change. This is because of the unique position the first FITS extension has in the FITS standard (for example it cannot be used to store tables).  File: gnuastro.info, Node: Keyword manipulation, Prev: HDU manipulation, Up: Invoking astfits 5.1.1.2 Keyword manipulation ............................ The meta-data in each header data unit, or HDU (also known as extension, see *note Fits::) is stored as “keywordâ€s. Each keyword consists of a name, value, unit, and comments. The Fits program (see *note Fits::) options related to viewing and manipulating keywords in a FITS HDU are described below. To see the full list of keywords in a FITS HDU, you can use the ‘--printallkeys’ option. If any of the keywords are to be modified, the headers of the input file will be changed. If you want to keep the original FITS file or HDU, it is easiest to create a copy first and then run Fits on that. In the FITS standard, keywords are always uppercase. So case does not matter in the input or output keyword names you specify. Most of the options can accept multiple instances in one command. For example you can add multiple keywords to delete by calling ‘--delete’ multiple times, since repeated keywords are allowed, you can even delete the same keyword multiple times. The action of such options will start from the top most keyword. The precedence of operations are described below. Note that while the order within each class of actions is preserved, the order of individual actions is not. So irrespective of what order you called ‘--delete’ and ‘--update’. First, all the delete operations are going to take effect then the update operations. 1. ‘--delete’ 2. ‘--rename’ 3. ‘--update’ 4. ‘--write’ 5. ‘--asis’ 6. ‘--history’ 7. ‘--comment’ 8. ‘--date’ 9. ‘--printallkeys’ All possible syntax errors will be reported before the keywords are actually written. FITS errors during any of these actions will be reported, but Fits won’t stop until all the operations are complete. If ‘--quitonerror’ is called, then Fits will immediately stop upon the first error. If you want to inspect only a certain set of header keywords, it is easiest to pipe the output of the Fits program to GNU Grep. Grep is a very powerful and advanced tool to search strings which is precisely made for such situations. For example if you only want to check the size of an image FITS HDU, you can run: $ astfits input.fits | grep NAXIS *FITS STANDARD KEYWORDS:* Some header keywords are necessary for later operations on a FITS file, for example BITPIX or NAXIS, see the FITS standard for their full list. If you modify (for example remove or rename) such keywords, the FITS file extension might not be usable any more. Also be careful for the world coordinate system keywords, if you modify or change their values, any future world coordinate system (like RA and Dec) measurements on the image will also change. The keyword related options to the Fits program are fully described below. ‘-a STR’ ‘--asis=STR’ Write ‘STR’ exactly into the FITS file header with no modifications. If it does not conform to the FITS standards, then it might cause trouble, so please be very careful with this option. If you want to define the keyword from scratch, it is best to use the ‘--write’ option (see below) and let CFITSIO worry about the standards. The best way to use this option is when you want to add a keyword from one FITS file to another unchanged and untouched. Below is an example of such a case that can be very useful sometimes (on the command-line or in scripts): $ key=$(astfits firstimage.fits | grep KEYWORD) $ astfits --asis="$key" secondimage.fits In particular note the double quotation signs (<">) around the reference to the ‘key’ shell variable (‘$key’), since FITS keywords usually have lots of space characters, if this variable is not quoted, the shell will only give the first word in the full keyword to this option, which will definitely be a non-standard FITS keyword and will make it hard to work on the file afterwords. See the “Quoting†section of the GNU Bash manual for more information if your keyword has the special characters <$>, <`>, or <\>. ‘-d STR’ ‘--delete=STR’ Delete one instance of the ‘STR’ keyword from the FITS header. Multiple instances of ‘--delete’ can be given (possibly even for the same keyword, when its repeated in the meta-data). All keywords given will be removed from the headers in the same given order. If the keyword doesn’t exist, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with ‘--quitonerror’. ‘-r STR’ ‘--rename=STR’ Rename a keyword to a new value. ‘STR’ contains both the existing and new names, which should be separated by either a comma (<,>) or a space character. Note that if you use a space character, you have to put the value to this option within double quotation marks (<">) so the space character is not interpreted as an option separator. Multiple instances of ‘--rename’ can be given in one command. The keywords will be renamed in the specified order. If the keyword doesn’t exist, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with ‘--quitonerror’. ‘-u STR’ ‘--update=STR’ Update a keyword, its value, its comments and its units in the format described below. If there are multiple instances of the keyword in the header, they will be changed from top to bottom (with multiple ‘--update’ options). The format of the values to this option can best be specified with an example: --update=KEYWORD,value,"comments for this keyword",unit If there is a writing error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with ‘--quitonerror’. The value can be any numerical or string value(1). Other than the ‘KEYWORD’, all the other values are optional. To leave a given token empty, follow the preceding comma (<,>) immediately with the next. If any space character is present around the commas, it will be considered part of the respective token. So if more than one token has space characters within it, the safest method to specify a value to this option is to put double quotation marks around each individual token that needs it. Note that without double quotation marks, space characters will be seen as option separators and can lead to undefined behavior. ‘-w STR’ ‘--write=STR’ Write a keyword to the header. For the possible value input formats, comments and units for the keyword, see the ‘--update’ option above. ‘-H STR’ ‘--history STR’ Add a ‘HISTORY’ keyword to the header. The string given to this keyword will be separated into multiple keyword cards if it is longer than 70 characters. With each run only one value for the ‘--history’ option will be read. If there are multiple, it is the last one. If there is an error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with ‘--quitonerror’. ‘-c STR’ ‘--comment STR’ Add a ‘COMMENT’ keyword to the header. Similar to the explanation for ‘--history’ above. If there is a writing error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with ‘--quitonerror’. ‘-t’ ‘--date’ Put the current date and time in the header. If the ‘DATE’ keyword already exists in the header, it will be updated. If there is a writing error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with ‘--quitonerror’. ‘-p’ ‘--printall’ Print all the keywords in the specified FITS extension (HDU) on the command-line. ‘-Q’ ‘--quitonerror’ Quit if any of the operations above are not successful. By default if an error occurs, Fits will warn the user of the faulty keyword and continue with the rest of actions. ---------- Footnotes ---------- (1) Some tricky situations arise with values like ‘‘87095e5’’, if this was intended to be a number it will be kept in the header as ‘8709500000’ and there is no problem. But this can also be a shortened Git commit hash. In the latter case, it should be treated as a string and stored as it is written. Commit hashes are very important in keeping the history of a file during your research and such values might arise without you noticing them in your reproduction pipeline. One solution is to use ‘git describe’ instead of the short hash alone. A less recommended solution is to add a space after the commit hash and Fits will write the value as ‘‘87095e5 ’’ in the header. If you later compare the strings on the shell, the space character will be ignored by the shell in the latter solution and there will be no problem.  File: gnuastro.info, Node: ConvertType, Next: Table, Prev: Fits, Up: Data containers 5.2 ConvertType =============== The formats of astronomical data were defined mainly for archiving and processing. In other situations, the data might be useful in other formats. For example, when you are writing a paper or report or if you are making slides for a talk, you can’t use a FITS image. Other image formats should be used. In other cases you might want your pixel values in a table format as plain text for input to other programs that don’t recognize FITS, or to include as a table in your report. ConvertType is created for such situations. The various types will increase with future updates and based on need. The conversion is not only one way (from FITS to other formats), but two ways (except the EPS and PDF formats). So you can convert a JPEG image or text file into a FITS image. Basically, other than EPS, you can use any of the recognized formats as different color channel inputs to get any of the recognized outputs. So before explaining the options and arguments, first a short description of the recognized files types will be given followed a short introduction to digital color. * Menu: * Recognized file formats:: Recognized file formats * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType.  File: gnuastro.info, Node: Recognized file formats, Next: Color, Prev: ConvertType, Up: ConvertType 5.2.1 Recognized file formats ----------------------------- The various standards and the file name extensions recognized by ConvertType are listed below. FITS or IMH Astronomical data are commonly stored in the FITS format (and in older data sets in IRAF ‘.imh’ format), a list of file name suffixes which indicate that the file is in this format is given in *note Arguments::. Each extension of a FITS image only has one value per pixel, so when used as input, each input FITS image contributes as one color channel. If you want multiple extensions in one FITS file for different color channels, you have to repeat the file name multiple times and use the ‘--hdu’, ‘--hdu2’, ‘--hdu3’ or ‘--hdu4’ options to specify the different extensions. JPEG The JPEG standard was created by the Joint photographic experts group. It is currently one of the most commonly used image formats. Its major advantage is the compression algorithm that is defined by the standard. Like the FITS standard, this is a raster graphics format, which means that it is pixelated. A JPEG file can have 1 (for gray-scale), 3 (for RGB) and 4 (for CMYK) color channels. If you only want to convert one JPEG image into other formats, there is no problem, however, if you want to use it in combination with other input files, make sure that the final number of color channels does not exceed four. If it does, then ConvertType will abort and notify you. The file name endings that are recognized as a JPEG file for input are: ‘.jpg’, ‘.JPG’, ‘.jpeg’, ‘.JPEG’, ‘.jpe’, ‘.jif’, ‘.jfif’ and ‘.jfi’. EPS The Encapsulated PostScript (EPS) format is essentially a one page PostScript file which has a specified size. PostScript also includes non-image data, for example lines and texts. It is a fully functional programming language to describe a document. Therefore in ConvertType, EPS is only an output format and cannot be used as input. Contrary to the FITS or JPEG formats, PostScript is not a raster format, but is categorized as vector graphics. The Portable Document Format (PDF) is currently the most common format for documents. Some believe that PDF has replaced PostScript and that PostScript is now obsolete. This view is wrong, a PostScript file is an actual plain text file that can be edited like any program source with any text editor. To be able to display its programmed content or print, it needs to pass through a processor or compiler. A PDF file can be thought of as the processed output of the compiler on an input PostScript file. PostScript, EPS and PDF were created and are registered by Adobe Systems. With these features in mind, you can see that when you are compiling a document with TeX or LaTeX, using an EPS file is much more low level than a JPEG and thus you have much greater control and therefore quality. Since it also includes vector graphic lines we also use such lines to make a thin border around the image to make its appearance in the document much better. No matter the resolution of the display or printer, these lines will always be clear and not pixelated. In the future, addition of text might be included (for example labels or object IDs) on the EPS output. However, this can be done better with tools within TeX or LaTeX such as PGF/Tikz(1). If the final input image (possibly after all operations on the flux explained below) is a binary image or only has two colors of black and white (in segmentation maps for example), then PostScript has another great advantage compared to other formats. It allows for 1 bit pixels (pixels with a value of 0 or 1), this can decrease the output file size by 8 times. So if a gray-scale image is binary, ConvertType will exploit this property in the EPS and PDF (see below) outputs. The standard formats for an EPS file are ‘.eps’, ‘.EPS’, ‘.epsf’ and ‘.epsi’. The EPS outputs of ConvertType have the ‘.eps’ suffix. PDF As explained above, a PDF document is a static document description format, viewing its result is therefore much faster and more efficient than PostScript. To create a PDF output, ConvertType will make a PostScript page description and convert that to PDF using GPL Ghostscript. The suffixes recognized for a PDF file are: ‘.pdf’, ‘.PDF’. If GPL Ghostscript cannot be run on the PostScript file, it will remain and a warning will be printed. ‘blank’ This is not actually a file type! But can be used to fill one color channel with a blank value. If this argument is given for any color channel, that channel will not be used in the output. Plain text Plain text files have the advantage that they can be viewed with any text editor or on the command-line. Most programs also support input as plain text files. As input, each plain text file is considered to contain one color channel. In ConvertType, the recognized extensions for plain text files are ‘.txt’ and ‘.dat’. As described in *note Invoking astconvertt::, if you just give these extensions, (and not a full filename) as output, then automatic output will be preformed to determine the final output name (see *note Automatic output::). Besides these, when the format of a file cannot be recognized from its name, ConvertType will fall back to plain text mode. So you can use any name (even without an extension) for a plain text input or output. Just note that when the suffix is not recognized, automatic output will not be preformed. The basic input/output on plain text images is very similar to how tables are read/written as described in *note Gnuastro text table format::. Simply put, the restrictions are very loose, and there is a convention to define a name, units, data type (see *note Numeric data types::), and comments for the data in a commented line. The only difference is that as a table, a text file can contain many datasets (columns), but as a 2D image, it can only contain one dataset. As a result, only one information comment line is necessary for a 2D image, and instead of the starting ‘‘# Column N’’ (‘N’ is the column number), the information line for a 2D image must start with ‘‘# Image 1’’. When ConvertType is asked to output to plain text file, this information comment line is written before the image pixel values. When converting an image to plain text, consider the fact that if the image is large, the number of columns in each line will become very large, possibly making it very hard to open in some text editors. Standard output (command-line) This is very similar to the plain text output, but instead of creating a file to keep the printed values, they are printed on the command line. This can be very useful when you want to redirect the results directly to another program in one command with no intermediate file. The only difference is that only the pixel values are printed (with no information comment line). To print to the standard output, set the output name to ‘‘stdout’’. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Color, Next: Invoking astconvertt, Prev: Recognized file formats, Up: ConvertType 5.2.2 Color ----------- An image is a two dimensional array of 2 dimensional elements called pixels. If each pixel only has one value, the image is known as a gray-scale image and no color is defined. The range of values in the image can be interpreted as shades of any color, it is customary to use shades of black or gray-scale. However, to produce the color spectrum in the digital world, several primary colors must be mixed. Therefore in a color image, each pixel has several values depending on how many primary colors were chosen. For example on the digital monitor or color digital cameras, all colors are built by mixing the three colors of Red-Green-Blue (RGB) with various proportions. However, for printing on paper, standard printers use the Cyan-Magenta-Yellow-Key (CMYK, Key=black) color space. Therefore when printing an RGB image, usually a transformation of color spaces will be necessary. In a colored digital camera, a color image is produced by dividing the pixel’s area between three colors (filters). However in astronomy due to the intrinsic faintness of most of the targets, the collecting area of the pixel is very important for us. Hence the full area of the pixel is used and one value is stored for that pixel in the end. One color filter is used for the whole image. Thus a FITS image is inherently a gray-scale image and no color can be defined for it. One way to represent a gray-scale image in different color spaces is to use the same proportions of the primary colors in each pixel. This is the common way most FITS image converters work: they fill all the channels with the same values. The downside is two fold: • Three (for RGB) or four (for CMYK) values have to be stored for every pixel, this makes the output file very heavy (in terms of bytes). • If printing, the printing errors of each color channel can make the printed image slightly more blurred than it actually is. To solve both these problems, the best way is to save the FITS image into the black channel of the CMYK color space. In the RGB color space all three channels have to be used. The JPEG standard is the only common standard that accepts CMYK color space, that is why currently only the JPEG standard is included and not the PNG standard for example. The JPEG and EPS standards set two sizes for the number of bits in each channel: 8-bit and 12-bit. The former is by far the most common and is what is used in ConvertType. Therefore, each channel should have values between 0 to 2^8-1=255. From this we see how each pixel in a gray-scale image is one byte (8 bits) long, in an RGB image, it is 3bytes long and in CMYK it is 4bytes long. But thanks to the JPEG compression algorithms, when all the pixels of one channel have the same value, that channel is compressed to one pixel. Therefore a Grayscale image and a CMYK image that has only the K-channel filled are approximately the same file size.  File: gnuastro.info, Node: Invoking astconvertt, Prev: Color, Up: ConvertType 5.2.3 Invoking ConvertType -------------------------- ConvertType will convert any recognized input file type to any specified output type. The executable name is ‘astconvertt’ with the following general template $ astconvertt [OPTION...] InputFile [InputFile2] ... [InputFile4] One line examples: ## Convert an image in FITS to PDF: $ astconvertt image.fits --output=pdf ## Convert an image in JPEG to FITS: $ astconvertt image.jpg -ogalaxy.fits ## Use three plain text 2D arrays to create an RGB JPEG output: $ astconvertt f1.txt f2.txt f3.fits -o.jpg ## Use two images and one blank for an RGB EPS output: $ astconvertt M31_r.fits M31_g.fits blank -oeps The file type of the output will be specified with the (possibly complete) file name given to the ‘--output’ option, which can either be given on the command-line or in any of the configuration files (see *note Configuration files::). Note that if the output suffix is not recognized, it will default to plain text format, see *note Recognized file formats::. The order of multiple input files is important. After reading the input file(s) the number of color channels in all the inputs will be used to define which color space is being used for the outputs and how each color channel is interpreted. Note that one file might have more than one color channel (for example in the JPEG format). If there is one color channel the output is gray-scale, if three input color channels are given they are respectively considered to be the red, green and blue color channels and if there are four color channels they are respectively considered to be cyan, magenta, yellow and black. The value to ‘--output’ (or ‘-o’) can be either a full file name or just the suffix of the desired output format. In the former case, that same name will be used for the output. In the latter case, the name of the output file will be set based on the automatic output guidelines, see *note Automatic output::. Note that the suffix name can optionally start a ‘.’ (dot), so for example ‘--output=.jpg’ and ‘--output=jpg’ are equivalent. See *note Recognized file formats:: Besides the common set of options explained in *note Common options::, the options to ConvertType can be classified into input, output and flux related options. The majority of the options are to do with the flux range. Astronomical data usually have a very large dynamic range (difference between maximum and minimum value) and different subjects might be better demonstrated with a limited flux range. Input: ‘-h STR/INT’ ‘--hdu=STR/INT’ In ConvertType, it is possible to call the HDU option multiple times for the different input FITS files (corresponding to different color channels) in the same order that they are called on the command-line. Except for the fact that multiple calls are possible, this option is identical to the common ‘--hdu’ in *note Input output options::. The number of calls to this option cannot be less than the number of input FITS files, but if there are more, the extra HDUs will be ignored, note that they will be read in the order described in *note Configuration file precedence::. Output: ‘-w FLT’ ‘--widthincm=FLT’ The width of the output in centimeters. This is only relevant for those formats that accept such a width (not plain text for example). For most digital purposes, the number of pixels is far more important than the value to this parameter because you can adjust the absolute width (in inches or centimeters) in your document preparation program. ‘-b INT’ ‘--borderwidth=INT’ The width of the border to be put around the EPS and PDF outputs in units of PostScript points. There are 72 or 28.35 PostScript points in an inch or centimeter respectively. In other words, there are roughly 3 PostScript points in every millimeter. If you are planning on adding a border, its significance is highly correlated with the value you give to the ‘--widthincm’ parameter. Unfortunately in the document structuring convention of the PostScript language, the “bounding box†has to be in units of PostScript points with no fractions allowed. So the border values only have to be specified in integers. To have a final border that is thinner than one PostScript point in your document, you can ask for a larger width in ConvertType and then scale down the output EPS or PDF file in your document preparation program. For example by setting ‘width’ in your ‘includegraphics’ command in TeX or LaTeX. Since it is vector graphics, the changes of size have no effect on the quality of your output quality (pixels don’t get different values). ‘-x’ ‘--hex’ Use Hexadecimal encoding in creating EPS output. By default the ASCII85 encoding is used which provides a much better compression ratio. When converted to PDF (or included in TeX or LaTeX which is finally saved as a PDF file), an efficient binary encoding is used which is far more efficient than both of them. The choice of EPS encoding will thus have no effect on the final PDF. So if you want to transfer your EPS files (for example if you want to submit your paper to arXiv or journals in PostScript), their storage might become important if you have large images or lots of small ones. By default ASCII85 encoding is used which offers a much better compression ratio (nearly 40 percent) compared to Hexadecimal encoding. ‘-u INT’ ‘--quality=INT’ The quality (compression) of the output JPEG file with values from 0 to 100 (inclusive). For other formats the value to this option is ignored. Note that only in gray-scale (when one input color channel is given) will this actually be the exact quality (each pixel will correspond to one input value). If it is in color mode, some degradation will occur. While the JPEG standard does support loss-less graphics, it is not commonly supported. Flux range: ‘-c STR’ ‘--chang=STR’ (‘=STR’) Change pixel values with the following format ‘"from1:to1, from2:to2,..."’. This option is very useful in displaying labeled pixels (not actual data images which have noise) like segmentation maps. In labeled images, usually a group of pixels have a fixed integer value. With this option, you can manipulate the labels before the image is displayed to get a better output for print or to emphasize on a particular set of labels and ignore the rest. The labels in the images will be changed in the same order given. By default first the pixel values will be converted then the pixel values will be truncated (see ‘--fluxlow’ and ‘--fluxhigh’). You can use any number for the values irrespective of your final output, your given values are stored and used in the double precision floating point format. So for example if your input image has labels from 1 to 20000 and you only want to display those with labels 957 and 11342 then you can run ConvertType with these options: $ astconvertt --change=957:50000,11342:50001 --fluxlow=5e4 \ --fluxhigh=1e5 segmentationmap.fits --output=jpg While the output JPEG format is only 8 bit, this operation is done in an intermediate step which is stored in double precision floating point. The pixel values are converted to 8-bit after all operations on the input fluxes have been complete. By placing the value in double quotes you can use as many spaces as you like for better readability. ‘-C’ ‘--changeaftertrunc’ Change pixel values (with ‘--change’) after truncation of the flux values, by default it is the opposite. ‘-L FLT’ ‘--fluxlow=FLT’ The minimum flux (pixel value) to display in the output image, any pixel value below this value will be set to this value in the output. If the value to this option is the same as ‘--fluxmax’, then no flux truncation will be applied. Note that when multiple channels are given, this value is used for all the color channels. ‘-H FLT’ ‘--fluxhigh=FLT’ The maximum flux (pixel value) to display in the output image, see ‘--fluxlow’. ‘-m INT’ ‘--maxbyte=INT’ This is only used for the JPEG and EPS output formats which have an 8-bit space for each channel of each pixel. The maximum value in each pixel can therefore be $2^8-1=255$. With this option you can change (decrease) the maximum value. By doing so you will decrease the dynamic range. It can be useful if you plan to use those values for other purposes. ‘-A INT’ ‘--flminbyte=INT’ If the lowest pixel value in the input channels is larger than the value to ‘--fluxlow’, then that input value will be redundant. In some situations it might be necessary to set the minimum byte value (0) to correspond to that flux even if the data do not reach that value. With this option you can do this. Note that if the minimum pixel value is smaller than ‘--fluxlow’, then this option is redundant. ‘-B INT’ ‘--fhmaxbyte=INT’ See ‘--flminbyte’. ‘-i’ ‘--invert’ For 8-bit output types (JPEG, EPS, and PDF for example) the final value that is stored is inverted so white becomes black and vice versa. The reason for this is that astronomical images usually have a very large area of blank sky in them. The result will be that a large are of the image will be black. Note that this behavior is ideal for gray-scale images, if you want a color image, the colors are going to be mixed up.  File: gnuastro.info, Node: Table, Prev: ConvertType, Up: Data containers 5.3 Table ========= Tables are the products of processing astronomical images and spectra. For example in Gnuastro, MakeCatalog will process the defined pixels over an object and produce a catalog (see *note MakeCatalog::). For each identified object, MakeCatalog can print its position on the image or sky, its total brightness and many other information that is deducible from the given image. Each one of these properties is a column in its output catalog (or table) and for each input object, we have a row. When there are only a small number of objects (rows) and not too many properties (columns), then a simple plain text file is mainly enough to store, transfer, or even use the produced data. However, to be more efficient in all these aspects, astronomers have defined the FITS binary table standard to store data in a binary (0 and 1) format, not plain text. This can offer major advantages in all those aspects: the file size will be greatly reduced and the reading and writing will be faster (because the RAM and CPU also work in binary). The FITS standard also defines a standard for ASCII tables, where the data are stored in the human readable ASCII format, but within the FITS file structure. These are mainly useful for keeping ASCII data along with images and possibly binary data as multiple (conceptually related) extensions within a FITS file. The acceptable table formats are fully described in *note Tables::. Binary tables are not easily readable by human eyes. There is no fixed/unified standard on how the zero and ones should be interpreted. The Unix-like operating systems have flourished because of a simple fact: communication between the various tools is based on human readable characters(1). So while the FITS table standards are very beneficial for the tools that recognize them, they are hard to use in the vast majority of available software. This creates limitations for their generic use. ‘Table’ is Gnuastro’s solution to this problem. With Table, FITS tables (ASCII or binary) are directly accessible to the Unix-like operating systems power-users (those working the command-line or shell, see *note Command-line interface::). With Table, a FITS table (in binary or ASCII formats) is only one command away from AWK (or any other tool you want to use). Just like a plain text file that you read with the ‘cat’ command. You can pipe the output of Table into any other tool for higher-level processing, see the examples in *note Invoking asttable:: for some simple examples. * Menu: * Invoking asttable:: Options and arguments to Table. ---------- Footnotes ---------- (1) In “The art of Unix programmingâ€, Eric Raymond makes this suggestion to programmers: “When you feel the urge to design a complex binary file format, or a complex binary application protocol, it is generally wise to lie down until the feeling passes.â€. This is a great book and strongly recommended, give it a look if you want to truly enjoy your work/life in this environment.  File: gnuastro.info, Node: Invoking asttable, Prev: Table, Up: Table 5.3.1 Invoking Table -------------------- Table will read/write, select, convert, or show the information of the columns in FITS ASCII table, FITS binary table and plain text table files, see *note Tables::. Output columns can also be determined by number or regular expression matching of column names, units, or comments. The executable name is ‘asttable’ with the following general template $ asttable [OPTION...] InputFile One line examples: ## Get the table column information (name, data type, or units): $ asttable bintab.fits --information ## Only print those columns which have a name starting with "MAG_": $ asttable bintab.fits --column=/^MAG_/ ## Only print the 2nd column, and the third column multiplied by 5: $ asttable bintab.fits | awk '{print $2, 5*$3}' ## Only print rows with a value in the 10th column above 100000: $ asttable bintab.fits | awk '$10>10e5 {print}' ## Sort the output columns by the third column, save output: $ asttable bintab.fits | 'sort -k3 > output.txt ## Convert a plain text table to a binary FITS table: $ asttable plaintext.txt --output=table.fits --tabletype=fits-binary In the absence of selected columns, all the input file’s columns will be output. If the specified output is a FITS file, the type of FITS table (binary or ASCII) will be determined from the ‘--tabletype’ option. If the output is not a FITS file, it will be printed as a plain text table (with space characters between the columns). When the columns are accompanied by meta-data (like column name, units, or comments), this information will also printed in the plain text file before the table, as described in *note Gnuastro text table format::. For the full list of options common to all Gnuastro programs please see *note Common options::. Options can also be stored in directory, user or system-wide configuration files to avoid repeating on the command-line, see *note Configuration files::. Table does not follow Automatic output that is common in most Gnuastro programs, see *note Automatic output::. Thus, in the absence of an output file, the selected columns will be printed on the command-line with no column information, ready for redirecting to other tools like AWK or sort, similar to the examples above. ‘-i’ ‘--information’ Only print the column information in the specified table on the command-line and exit. Each column’s information (number, name, units, data type, and comments) will be printed as a row on the command-line. Note that the FITS standard only requires the data type (see *note Numeric data types::), and in plain text tables, no meta-data/information is mandatory. Gnuastro has its own convention in the comments of a plain text table to store and transfer this information as described in *note Gnuastro text table format::. This option will take precedence over the ‘--column’ option, so when it is called along with requested columns, the latter will be ignored. This can be useful if you forget the identifier of a column after you have already typed some on the command-line. You can simply add a ‘-i’ and run Table to see the whole list and remember. Then you can use the shell history (with the up arrow key on the keyboard), and retrieve the last command with all the previously typed columns present, delete ‘-i’ and add the identifier you had forgot. ‘-c STR/INT’ ‘--column=STR/INT’ Specify the columns to output, see *note Selecting table columns:: for a thorough explanation on how the value to this option is interpreted. To select several output columns, this option can also be called any number times in one call to Table. The order of the output columns will be the same call order on the command-line. This option is not mandatory, if no specific columns are requested, all the input table columns are output. When this option is called multiple times, it is possible to output one column more than once.  File: gnuastro.info, Node: Data manipulation, Next: Data analysis, Prev: Data containers, Up: Top 6 Data manipulation ******************* Images are one of the major formats of data that is used in astronomy. The functions in this chapter explain the GNU Astronomy Utilities which are provided for their manipulation. For example cropping out a part of a larger image or convolving the image with a given kernel or applying a transformation to it. * Menu: * Crop:: Crop region(s) from a dataset. * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * Warp:: Warp/Transform an image to a different grid.  File: gnuastro.info, Node: Crop, Next: Arithmetic, Prev: Data manipulation, Up: Data manipulation 6.1 Crop ======== Astronomical images are often very large, filled with thousands of galaxies. It often happens that you only want a section of the image, or you have a catalog of sources and you want to visually analyze them in small postage stamps. Crop is made to do all these things. When more than one crop is required, Crop will divide the crops between multiple threads to significantly reduce the run time. Astronomical surveys are usually extremely large. So large in fact, that the whole survey will not fit into a reasonably sized file. Because of this, surveys usually cut the final image into separate tiles and store each tile in a file. For example the COSMOS survey’s Hubble space telescope, ACS F814W image consists of 81 separate FITS images, with each one having a volume of 1.7 Giga bytes. Even though the tile sizes are chosen to be large enough that too many galaxies/targets don’t fall on the edges of the tiles, inevitably some do. So when you simply crop the image of such targets from one tile, you will miss a large area of the surrounding sky (which is essential in estimating the noise). Therefore in its WCS mode, Crop will stitch parts of the tiles that are relevant for a target (with the given width) from all the input images that cover that region into the output. Of course, the tiles have to be present in the list of input files. Besides cropping postage stamps around certain coordinates, Crop can also crop arbitrary polygons from an image (or a set of tiles by stitching the relevant parts of different tiles within the polygon), see ‘--polygon’ in *note Invoking astcrop::. Alternatively, it can crop out rectangular regions through the ‘--section’ option from one image, see *note Crop section syntax::. * Menu: * Crop modes:: Basic modes to define crop region. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astcrop:: Calling Crop on the command-line  File: gnuastro.info, Node: Crop modes, Next: Crop section syntax, Prev: Crop, Up: Crop 6.1.1 Crop modes ---------------- In order to be comprehensive, intuitive, and easy to use, there are two ways to define the crop: 1. From its center and side length. For example if you already know the coordinates of an object and want to inspect it in an image or to generate postage stamps of a catalog containing many such coordinates. 2. The vertices of the crop region, this can be useful for larger crops over many targets, for example to crop out a uniformly deep, or contiguous, region of a large survey. Irrespective of how the crop region is defined, the coordinates to define the crop can be in Image (pixel) or World Coordinate System (WCS) standards. All coordinates are read as floating point numbers (not integers, except for the ‘--section’ option, see below). By setting the _mode_ in Crop, you define the standard that the given coordinates must be interpretted. Here, the different ways to specify the crop region are discussed within each standard. For the full list options, please see *note Invoking astcrop::. When the crop is defined by its center, the respective (integer) central pixel position will be found internally according to the FITS standard. To have this pixel positioned in the center of the cropped region, the final cropped region will have an add number of pixels (even if you give an even number to ‘--width’ in image mode). Furthermore, when the crop is defined as by its center, Crop allows you to only keep crops what don’t have any blank pixels in the vicinity of their center (your primary target). This can be very convenient when your input catalog/coordinates originated from another survey/filter which is not fully covered by your input image, to learn more about this feature, please see the description of the ‘--checkcenter’ option in *note Invoking astcrop::. Image coordinates In image mode (‘--mode=img’), Crop interprets the pixel coordinates and widths in units of the input data-elements (for example pixels in an image, not world coordinates). In image mode, only one image may be input. The output crop(s) can be defined in multiple ways as listed below. Center of multiple crops (in a catalog) The center of (possibly multiple) crops are read from a text file. In this mode, the columns identified with the ‘--coordcol’ option are interpreted as the center of a crop with a width of ‘--width’ pixels along each dimension. The columns can contain any floating point value. The value to ‘--output’ option is seen as a directory which will host (the possibly multiple) separate crop files, see *note Crop output:: for more. For a tutorial using this feature, please see *note Hubble visually checks and classifies his catalog::. Center of a single crop (on the command-line) The center of the crop is given on the command-line with the ‘--center’ option. The crop width is specified by the ‘--width’ option along each dimension. The given coordinates and width can be any floating point number. Vertices of a single crop In Image mode there are two options to define the vertices of a region to crop: ‘--section’ and ‘--polygon’. The former is lower-level (doesn’t accept floating point vertices, and only a rectangular region can be defined), it is also only available in Image mode. Please see *note Crop section syntax:: for a full description of this method. The latter option (‘--polygon’) is a higher-level method to define any convex polygon (with any number of vertices) with floating point values. Please see the description of this option in *note Invoking astcrop:: for its syntax. WCS coordinates In WCS mode (‘--mode=wcs’), the coordinates and widths are interpretted using the World Coordinate System (WCS, that must accompany the dataset), not pixel coordinates. In WCS mode, Crop accepts multiple datasets as input. When the cropped region (defined by its center or vertices) overlaps with multiple of the input images/tiles, the overlapping regions will be taken from the respective input (they will be stitched when necessary for each output crop). In this mode, the input images do not necessarily have to be the same size, they just need to have the same orientation and pixel resolution. Currently only orientation along the celestial coordinates is accepted, if your input has a different orientation you can use Warp’s ‘--align’ option to align the image before cropping it (see *note Warp::). Each individual input image/tile can even be smaller than the final crop. In any case, any part of any of the input images which overlaps with the desired region will be used in the crop. Note that if there is an overlap in the input images/tiles, the pixels from the last input image read are going to be used for the overlap. Crop will not change pixel values, so it assumes your overlapping tiles were cutout from the same original image. There are multiple ways to define your cropped region as listed below. Center of multiple crops (in a catalog) Similar to catalog inputs in Image mode (above), except that the values along each dimension are assumed to have the same units as the dataset’s WCS information. For example, the central RA and Dec value for each crop will be read from the first and second calls to the ‘--coordcol’ option. The width of the cropped box (in units of the WCS, or degrees in RA and Dec mode) must be specified with the ‘--width’ option. Center of a single crop (on the command-line) You can specify the center of only one crop box with the ‘--center’ option. If it exists in the input images, it will be cropped similar to the catalog mode, see above also for ‘--width’. Vertices of a single crop The ‘--polygon’ option is a high-level method to define any convex polygon (with any number of vertices). Please see the description of this option in *note Invoking astcrop:: for its syntax. *CAUTION:* In WCS mode, the image has to be aligned with the celestial coordinates, such that the first FITS axis is parallel (opposite direction) to the Right Ascension (RA) and the second FITS axis is parallel to the declination. If these conditions aren’t met for an image, Crop will warn you and abort. You can use Warp’s ‘--align’ option to align the input image with these coordinates, see *note Warp::. As a summary, if you don’t specify a catalog, you have to define the cropped region manually on the command-line. In any case the mode is mandatory for Crop to be able to interpret the values given as coordinates or widths.  File: gnuastro.info, Node: Crop section syntax, Next: Blank pixels, Prev: Crop modes, Up: Crop 6.1.2 Crop section syntax ------------------------- When in image mode, one of the methods to crop only one rectangular section from the input image is to use the ‘--section’ option. Crop has a powerful syntax to read the box parameters from a string of characters. If you leave certain parts of the string to be empty, Crop can fill them for you based on the input image sizes. To define a box, you need the coordinates of two points: the first (‘X1’, ‘Y1’) and the last pixel (‘X2’, ‘Y2’) pixel positions in the image, or four integer numbers in total. The four coordinates can be specified with one string in this format: ‘‘X1:X2,Y1:Y2’’. This string is given to the ‘--section’ option. Therefore, the pixels along the first axis that are $\geq$‘X1’ and $\leq$‘X2’ will be included in the cropped image. The same goes for the second axis. Note that each different term will be read as an integer, not a float. This is a low-level option, for a higher-level way to specify region (any polygon, not just a box), please see the ‘--polygon’ option in *note Crop options::. Also note that in the FITS standard, pixel indexes along each axis start from unity(1) not zero(0). You can omit any of the values and they will be filled automatically. The left hand side of the colon (‘:’) will be filled with ‘1’, and the right side with the image size. So, ‘2:,:’ will include the full range of pixels along the second axis and only those with a first axis index larger than ‘2’ in the first axis. If the colon is omitted for a dimension, then the full range is automatically used. So the same string is also equal to ‘2:,’ or ‘2:’ or even ‘2’. If you want such a case for the second axis, you should set it to: ‘,2’. If you specify a negative value, it will be seen as before the indexes of the image which are outside the image along the bottom or left sides when viewed in SAO ds9. In case you want to count from the top or right sides of the image, you can use an asterisk (‘*’). When confronted with a ‘*’, Crop will replace it with the maximum length of the image in that dimension. So ‘*-10:*+10,*-20:*+20’ will mean that the crop box will be 20\times40 pixels in size and only include the top corner of the input image with 3/4 of the image being covered by blank pixels, see *note Blank pixels::. If you feel more comfortable with space characters between the values, you can use as many space characters as you wish, just be careful to put your value in double quotes, for example ‘--section="5:200, 123:854"’. If you forget the quotes, anything after the first space will not be seen by ‘--section’ and you will most probably get an error because the rest of your string will be read as a filename (which most probably doesn’t exist). See *note Command-line:: for a description of how the command-line works.  File: gnuastro.info, Node: Blank pixels, Next: Invoking astcrop, Prev: Crop section syntax, Up: Crop 6.1.3 Blank pixels ------------------ The cropped box can potentially include pixels that are beyond the image range. For example when a target in the input catalog was very near the edge of the input image. The parts of the cropped image that were not in the input image will be filled with the following two values depending on the data type of the image. In both cases, SAO ds9 will not color code those pixels. • If the data type of the image is a floating point type (float or double), IEEE NaN (Not a number) will be used. • For integer types, pixels out of the image will be filled with the value of the ‘BLANK’ keyword in the cropped image header. The value assigned to it is the lowest value possible for that type, so you will probably never need it any way. Only for the unsigned character type (‘BITPIX=8’ in the FITS header), the maximum value is used because it is unsigned, the smallest value is zero which is often meaningful. You can ask for such blank regions to not be included in the output crop image using the ‘--noblank’ option. In such cases, there is no guarantee that the image size of your outputs are what you asked for. In some survey images, unfortunately they do not use the ‘BLANK’ FITS keyword. Instead they just give all pixels outside of the survey area a value of zero. So by default, when dealing with float or double image types, any values that are 0.0 are also regarded as blank regions. This can be turned off with the ‘--zeroisnotblank’ option.  File: gnuastro.info, Node: Invoking astcrop, Prev: Blank pixels, Up: Crop 6.1.4 Invoking Crop ------------------- Crop will crop a region from an image. If in WCS mode, it will also stitch parts from separate images in the input files. The executable name is ‘astcrop’ with the following general template $ astcrop [OPTION...] [ASCIIcatalog] ASTRdata ... One line examples: ## Crop all objects in cat.txt from image.fits: $ astcrop --catalog=cat.txt image.fits ## Crop all options in catalog (with RA,DEC) from all the files ## ending in `_drz.fits' in `/mnt/data/COSMOS/': $ astcrop --mode=wcs --catalog=cat.txt /mnt/data/COSMOS/*_drz.fits ## Crop the outer 10 border pixels of the input image: $ astcrop --section=10:*-10,10:*-10 --hdu=2 image.fits ## Crop region around RA and Dec of (189.16704, 62.218203): $ astcrop --mode=wcs --center=189.16704,62.218203 goodsnorth.fits ## Crop region around pixel coordinate (568.342, 2091.719): $ astcrop --mode=img --center=568.342,2091.719 --width=201 image.fits Crop has one mandatory argument which is the input image name(s), shown above with ‘ASTRdata ...’. You can use shell expansions, for example ‘*’ for this if you have lots of images in WCS mode. If the crop box centers are in a catalog, you can use the ‘--catalog’ option. In other cases, you have to provide the single cropped output parameters must be given with command-line options. See *note Crop output:: for how the output file name(s) can be specified. For the full list of general options to all Gnuastro programs (including Crop), please see *note Common options::. Floating point numbers can be used to specify the crop region (except the ‘--section’ option, see *note Crop section syntax::). In such cases, the floating point values will be used to find the desired integer pixel indices based on the FITS standard. Hence, Crop ultimately doesn’t do any sub-pixel cropping (in other words, it doesn’t change pixel values). If you need such crops, you can use *note Warp:: to first warp the image to the a new pixel grid, then crop from that. For example, let’s assume you want a crop from pixels 12.982 to 80.982 along the first dimension. You should first translate the image by $-0.482$ (note that the edge of a pixel is at integer multiples of $0.5$). So you should run Warp with ‘--translate=-0.482,0’ and then crop the warped image with ‘--section=13:81’. There are two ways to define the cropped region: with its center or its vertices. See *note Crop modes:: for a full description. In the former case, Crop can check if the central region of the cropped image is indeed filled with data or is blank (see *note Blank pixels::), and not produce any output when the center is blank, see the description under ‘--checkcenter’ for more. When in catalog mode, Crop will run in parallel unless you set ‘--numthreads=1’, see *note Multi-threaded operations::. Note that when multiple outputs are created with threads, the outputs will not be created in the same order. This is because the threads are asynchronous and thus not started in order. This has no effect on each output, see *note Hubble visually checks and classifies his catalog:: for a tutorial on effectively using this feature. * Menu: * Crop options:: A list of all the options with explanation. * Crop output:: The outputs of Crop.  File: gnuastro.info, Node: Crop options, Next: Crop output, Prev: Invoking astcrop, Up: Invoking astcrop 6.1.4.1 Crop options .................... The options can be classified into the following contexts: Input, Output and operating mode options. Options that are common to all Gnuastro program are listed in *note Common options:: and will not be repeated here. When you are specifying the crop vertices your self (through ‘--section’, or ‘--polygon’) on relatively small regions (depending on the resolution of your images) the outputs from image and WCS mode can be approximately equivalent. However, as the crop sizes get large, the curved nature of the WCS coordinates have to be considered. For example, when using ‘--section’, the right ascension of the bottom left and top left corners will not be equal. If you only want regions within a given right ascension, use ‘--polygon’ in WCS mode. Input image parameters: ‘--hstartwcs=INT’ Specify the first keyword card (line number) to start finding the input image world coordinate system information. Distortions were only recently included in WCSLIB (from version 5). Therefore until now, different telescope would apply their own specific set of WCS keywords and put them into the image header along with those that WCSLIB does recognize. So now that WCSLIB recognizes most of the standard distortion parameters, they will get confused with the old ones and give completely wrong results. For example in the CANDELS-GOODS South images(1). The two ‘--hstartwcs’ and ‘--hendwcs’ are thus provided so when using older datasets, you can specify what region in the FITS headers you want to use to read the WCS keywords. Note that this is only relevant for reading the WCS information, basic data information like the image size are read separately. These two options will only be considered when the value to ‘--hendwcs’ is larger than that of ‘--hstartwcs’. So if they are equal or ‘--hstartwcs’ is larger than ‘--hendwcs’, then all the input keywords will be parsed to get the WCS information of the image. ‘--hendwcs=INT’ Specify the last keyword card to read for specifying the image world coordinate system on the input images. See ‘--hstartwcs’ Crop box parameters: ‘-c FLT[,FLT[,...]]’ ‘--center=FLT[,FLT[,...]]’ The central position of the crop in the input image. The positions along each dimension must be separated by a comma (<,>) and fractions are also acceptable. The number of values given to this option must be the same as the dimensions of the input dataset. The width of the crop should be set with ‘--width’. The units of the coordinates are read based on the value to the ‘--mode’ option, see below. ‘-w FLT[,FLT[,...]]’ ‘--width=FLT[,FLT[,...]]’ Width of the cropped region about its center. ‘--width’ may take either a single value (to be used for all dimensions) or multiple values (a specific value for each dimension). If in WCS mode, value(s) given to this option will be read in the same units as the dataset’s WCS information along this dimension. The final output will have an odd number of pixels to allow easy identification of the pixel which keeps your requested coordinate (from ‘--center’ or ‘--catalog’). The ‘--width’ option also accepts fractions. For example if you want the width of your crop to be 3 by 5 arcseconds along RA and Dec respectively, you can call it with: ‘--width=3/3600,5/3600’. If you want an even sided crop, you can run Crop afterwards with ‘--section=":*-1,:*-1"’ or ‘--section=2:,2:’ (depending on which side you don’t need), see *note Crop section syntax::. ‘-l STR’ ‘--polygon=STR’ String of crop polygon vertices. Note that currently only convex polygons should be used. In the future we will make it work for all kinds of polygons. Convex polygons are polygons that do not have an internal angle more than 180 degrees. This option can be used both in the image and WCS modes, see *note Crop modes::. The cropped image will be the size of the rectangular region that completely encompasses the polygon. By default all the pixels that are outside of the polygon will be set as blank values (see *note Blank pixels::). However, if ‘--outpolygon’ is called all pixels internal to the vertices will be set to blank. The syntax for the polygon vertices is similar to, and simpler than, that for ‘--section’. In short, the dimensions of each coordinate are separated by a comma (<,>) and each vertex is separated by a colon (<:>). You can define as many vertices as you like. If you would like to use space characters between the dimensions and vertices to make them more human-readable, then you have to put the value to this option in double quotation marks. For example, let’s assume you want to work on the deepest part of the WFC3/IR images of Hubble Space Telescope eXtreme Deep Field (HST-XDF). According to the webpage (https://archive.stsci.edu/prepds/xdf/)(2) the deepest part is contained within the coordinates: [ (53.187414,-27.779152), (53.159507,-27.759633), (53.134517,-27.787144), (53.161906,-27.807208) ] They have provided mask images with only these pixels in the WFC3/IR images, but what if you also need to work on the same region in the full resolution ACS images? Also what if you want to use the CANDELS data for the shallow region? Running Crop with ‘--polygon’ will easily pull out this region of the image for you irrespective of the resolution. If you have set the operating mode to WCS mode in your nearest configuration file (see *note Configuration files::), there is no need to call ‘--mode=wcs’ on the command line. You may also provide many FITS images/tiles and Crop will stitch them to produce this cropped region: $ astcrop --mode=wcs desired-filter-image(s).fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" In other cases, you have an image and want to define the polygon yourself (it isn’t already published like the example above). As the number of vertices increases, checking the vertex coordinates on a FITS viewer (for example SAO ds9) and typing them in one by one can be very tedious and prone to typo errors. You can take the following steps to avoid the frustration and possible typos: Open the image with ds9 and activate its “region†mode with Edit→Region. Then define the region as a polygon with Region→Shape→Polygon. Click on the approximate center of the region you want and a small square will appear. By clicking on the vertices of the square you can shrink or expand it, clicking and dragging anywhere on the edges will enable you to define a new vertex. After the region has been nicely defined, save it as a file with Region→Save Regions. You can then select the name and address of the output file, keep the format as ‘REG’ and press “OKâ€. In the next window, keep format as “ds9†and “Coordinate System†as “fk5â€. A plain text file (let’s call it ‘ds9.reg’) is now created. You can now convert this plain text file to Crop’s polygon format with this command (when typing on the command-line, ignore the “<\>†at the end of the first and second lines along with the extra spaces, these are only for nice printing): $ v=$(awk 'NR==4' ds9.reg | sed -e's/polygon(//' \ -e's/\([^,]*,[^,]*\),/\1:/g' -e's/)//' ) $ astcrop --mode=wcs image.fits --polygon=$v ‘--outpolygon’ Keep all the regions outside the polygon and mask the inner ones with blank pixels (see *note Blank pixels::). This is practically the inverse of the default mode of treating polygons. Note that this option only works when you have only provided one input image. If multiple images are given (in WCS mode), then the full area covered by all the images has to be shown and the polygon excluded. This can lead to a very large area if large surveys like COSMOS are used. So Crop will abort and notify you. In such cases, it is best to crop out the larger region you want, then mask the smaller region with this option. ‘-s STR’ ‘--section=STR’ Section of the input image which you want to be cropped. See *note Crop section syntax:: for a complete explanation on the syntax required for this input. ‘-x STR/INT’ ‘--coordcol=STR/INT’ The column in a catalog to read as a coordinate. The value can be either the column number (starting from 1), or a match/search in the table meta-data, see *note Selecting table columns::. This option must be called multiple times, depending on the number of dimensions in the input dataset. If it is called more than necessary, the extra columns (later calls to this option on the command-line or configuration files) will be ignored, see *note Configuration file precedence::. ‘-n STR/INT’ ‘--namecol=STR/INT’ Column selection of crop file name. The value can be either the column number (starting from 1), or a match/search in the table meta-data, see *note Selecting table columns::. This option can be used both in Image and WCS modes, and not a mandatory. When a column is given to this option, the final crop base file name will be taken from the contents of this column. The directory will be determined by the ‘--output’ option (current directory if not given) and the value to ‘--suffix’ will be appended. When this column isn’t given, the row number will be used instead. Output options: ‘-c INT’ ‘--checkcenter=INT’ Box width (odd number of pixels) of region in the center of the image to check for blank values. If the value to this option is zero, no checking is done. This option is only relevant when the cropped region(s) are defined by their center (not by the vertices, see *note Crop modes::). If any of the pixels in this central region of a crop (defined by its center) are blank, then it will not be created. Because survey regions don’t often have a clean square or rectangle shape, some of the pixels on the sides of the survey FITS image don’t commonly have any data and are blank (see *note Blank pixels::). So when the catalog was not generated from the input image, it often happens that the image does not have data over some of the points. When the given center of a crop falls in such regions and this option has a non-zero, odd value, no crop will be created. Therefore with this option, you can specify a width of a small box (3 pixels is often good enough) around the central pixel of the cropped image. You can check which crops were created and which weren’t from the command-line (if ‘--quiet’ was not called, see *note Operating mode options::), or in Crop’s log file (see *note Crop output::). ‘-p STR’ ‘--suffix=STR’ The suffix (or post-fix) of the output files for when you want all the cropped images to have a special ending. One case where this might be helpful is when besides the science images, you want the weight images (or exposure maps, which are also distributed with survey images) of the cropped regions too. So in one run, you can set the input images to the science images and ‘--suffix=_s.fits’. In the next run you can set the weight images as input and ‘--suffix=_w.fits’. ‘-b’ ‘--noblank’ Pixels outside of the input image that are in the crop box will not be used. By default they are filled with blank values (depending on type), see *note Blank pixels::. This option only applies only in Image mode, see *note Crop modes::. ‘-z’ ‘--zeroisnotblank’ In float or double images, it is common to give the value of zero to blank pixels. If the input image type is one of these two types, such pixels will also be considered as blank. You can disable this behavior with this option, see *note Blank pixels::. Operating mode options: ‘-O STR’ ‘--mode=STR’ Operate in Image mode or WCS mode when the input coordinates can be both image or WCS. The value must either be ‘img’ or ‘wcs’, see *note Crop modes:: for a full description. ---------- Footnotes ---------- (1) (2)  File: gnuastro.info, Node: Crop output, Prev: Crop options, Up: Invoking astcrop 6.1.4.2 Crop output ................... The string given to ‘--output’ option will be interpretted depending on how many crops were requested, see *note Crop modes::: • When a catalog is given, the value of the ‘--output’ (see *note Common options::) will be read as the directory to store the output cropped images. Hence if it doesn’t already exist, Crop will abort with an error of a “No such file or directory†error. The crop file names will consist of two parts: a variable part (the row number of each target starting from 1) along with a fixed string which you can set with the ‘--suffix’ option. Optionally, you may also use the ‘--namecol’ option to define a column in the input catalog to use as the file name instead of numbers. • When only one crop is desired, the value to ‘--output’ will be read as a file name. If no output is specified or if it is a directory, the output file name will follow the automatic output names of Gnuastro, see *note Automatic output::: The string given to ‘--suffix’ will be replaced with the ‘.fits’ suffix of the input. The header of each output cropped image will contain the names of the input image(s) it was cut from. If a name is longer than the 70 character space that the FITS standard allows for header keyword values, the name will be cut into several keywords from the nearest slash (). The keywords have the following format: ‘ICFn_m’ (for Crop File). Where ‘n’ is the number of the image used in this crop and ‘m’ is the part of the name (it can be broken into multiple keywords). Following the name is another keyword named ‘ICFnPIX’ which shows the pixel range from that input image in the same syntax as *note Crop section syntax::. So this string can be directly given to the ‘--section’ option later. Once done, a log file can be created in the current directory with the ‘--log’ option. This file will have three columns and the same number of rows as the number of cropped images. There are also comments on the top of the log file explaining basic information about the run and descriptions for the columns. A short description of the columns is also given below: 1. The cropped image file name for that row. 2. The number of input images that were used to create that image. 3. A ‘0’ if the central few pixels (value to the ‘--checkcenter’ option) are blank and ‘1’ if they aren’t. When the crop was not defined by its center (see *note Crop modes::), or ‘--checkcenter’ was given a value of 0 (see *note Invoking astcrop::), the center will not be checked and this column will be given a value of ‘-1’.  File: gnuastro.info, Node: Arithmetic, Next: Convolve, Prev: Crop, Up: Data manipulation 6.2 Arithmetic ============== It is commonly necessary to do operations on some or all of the elements of a dataset independently (pixels in an image). For example, in the reduction of raw data it is necessary to subtract the Sky value (*note Sky value::) from each image image. Later (once the images as warped into a single grid using Warp for example, see *note Warp::), the images are co-added (the output pixel grid is the average of the pixels of the individual input images). Arithmetic is Gnuastro’s program for such operations on your datasets directly from the command-line. It currently uses the reverse polish or post-fix notation, see *note Reverse polish notation:: and will work on the native data types of the input images/data to reduce CPU and RAM resources, see *note Numeric data types::. For more information on how to run Arithmetic, please see *note Invoking astarithmetic::. * Menu: * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output  File: gnuastro.info, Node: Reverse polish notation, Next: Arithmetic operators, Prev: Arithmetic, Up: Arithmetic 6.2.1 Reverse polish notation ----------------------------- The most common notation for arithmetic operations is the infix notation (https://en.wikipedia.org/wiki/Infix_notation) where the operator goes between the two operands, for example $4+5$. While the infix notation is the preferred way in most programming languages, currently Arithmetic does not use it since it will require parenthesis which can complicate the implementation of the code. In the near future we do plan to adopt this notation(1), but for the time being (due to time constraints on the developers), Arithmetic uses the post-fix or reverse polish notation (https://en.wikipedia.org/wiki/Reverse_Polish_notation). The Wikipedia article provides some excellent explanation on this notation but here we will give a short summary here for self-sufficiency. In the post-fix notation, the operator is placed after the operands, as we will see below this removes the need to define parenthesis for most ordinary operators. For example, instead of writing ‘5+6’, we write ‘5 6 +’. To easily understand how this notation works, you can think of each operand as a node in a first-in-first-out stack. Every time an operator is confronted, it pops the number of operands it needs from the top of the stack (so they don’t exist in the stack any more), does its operation and pushes the result back on top of the stack. So if you want the average of 5 and 6, you would write: ‘5 6 + 2 /’. The operations that are done are: 1. ‘5’ is an operand, so it is pushed to the top of the stack. 2. ‘6’ is an operand, so it is pushed to the top of the stack. 3. ‘+’ is a binary operator, so pull the top two elements of the stack and perform addition on them (the order is $5+6$ in the example above). The result is ‘11’, push it on top of the stack. 4. ‘2’ is an operand so push it onto the top of the stack. 5. ‘/’ is a binary operator, so pull out the top two elements of the stack (top-most is ‘2’, then ‘11’) and divide the second one by the first. In the Arithmetic program, the operands can be FITS images or numbers. As you can see, very complicated procedures can be created without the need for parenthesis or worrying about precedence. Even functions which take an arbitrary number of arguments can be defined in this notation. This is a very powerful notation and is used in languages like Postscript (2) (the programming language in Postscript and compiled into PDF files) uses this notation. ---------- Footnotes ---------- (1) (2) See the EPS and PDF part of *note Recognized file formats:: for a little more on the Postscript language.  File: gnuastro.info, Node: Arithmetic operators, Next: Invoking astarithmetic, Prev: Reverse polish notation, Up: Arithmetic 6.2.2 Arithmetic operators -------------------------- The recognized operators in Arithmetic are listed below. See *note Reverse polish notation:: for more on how the operators and operands should be ordered on the command-line. The operands to all operators can be a data array (for example a FITS image) or a number, the output will be an array or number according to the inputs. For example a number multiplied by an array will produce an array. The conditional operators will return pixel, or numerical values of 0 (false) or 1 (true) and stored in an ‘unsigned char’ data type (see *note Numeric data types::). ‘+’ Addition, so “‘4 5 +’†is equivalent to $4+5$. ‘-’ Subtraction, so “‘4 5 -’†is equivalent to $4-5$. ‘x’ Multiplication, so “‘4 5 x’†is equivalent to $4\times5$. ‘/’ Division, so “‘4 5 /’†is equivalent to $4/5$. ‘%’ Modulo (remainder), so “‘3 2 %’†is equivalent to $1$. Note that the modulo operator only works on integer types. ‘abs’ Absolute value of first operand, so “‘4 abs’†is equivalent to $|4|$. ‘pow’ First operand to the power of the second, so “‘4.3 5f pow’†is equivalent to $4.3^{5}$. Currently ‘pow’ will only work on single or double precision floating point numbers or images. To be sure that a number is read as a floating point (even if it doesn’t have any non-zero decimals) put an ‘f’ after it. ‘sqrt’ The square root of the first operand, so “‘5 sqrt’†is equivalent to $\sqrt{5}$. The output type is determined from the input, so the output of this example will be ‘2’ (since ‘5’ doesn’t have any non-zero decimal digits). If you want ‘2.23607’, run ‘5f sqrt’ instead, the ‘f’ will ensure that a number will be read as a floating point number, even if it doesn’t have decimal digits. If the input image has an integer type, you should explicitly convert the image to floating point, for example ‘a.fits float sqrt’, see the type conversion operators below. ‘log’ Natural logarithm of first operand, so “‘4 log’†is equivalent to $\ln(4)$. The output type is determined from the input, see the explanation under ‘sqrt’ for more. ‘log10’ Base-10 logarithm of first operand, so “‘4 log10’†is equivalent to $\log(4)$. The output type is determined from the input, see the explanation under ‘sqrt’ for more. ‘minvalue’ Minimum (non-blank) value in the top operand on the stack, so “‘a.fits minvalue’†will push the the minimum pixel value in this image onto the stack. Therefore this operator is mainly intended for data (for example images), if the top operand is a number, this operator just returns it without any change. So note that when this operator acts on a single image, the output will no longer be an image, but a number. The output of this operand is in the same type as the input. ‘maxvalue’ Maximum (non-blank) value of first operand in the same type, similar to ‘minvalue’. ‘numvalue’ Number of non-blank elements in first operand in the ‘uint64’ type, similar to ‘minvalue’. ‘sumvalue’ Sum of non-blank elements in first operand in the ‘float32’ type, similar to ‘minvalue’. ‘meanvalue’ Mean value of non-blank elements in first operand in the ‘float32’ type, similar to ‘minvalue’. ‘stdvalue’ Standard deviation of non-blank elements in first operand in the ‘float32’ type, similar to ‘minvalue’. ‘medianvalue’ Median of non-blank elements in first operand with the same type, similar to ‘minvalue’. ‘min’ The first popped operand to this operator must be a positive integer number which specifies how many further operands should be popped from the stack. The given number of operands must have the same type and size. Each pixel of the output of this operator will be set to the minimum value of the given number of operands (images) in that pixel. For example the following command will produce an image with the same size and type as the inputs but each output pixel is set to the minimum respective pixel value of the three input images. $ astarithmetic a.fits b.fits c.fits 3 min Important notes: • NaN/blank pixels will be ignored, see *note Blank pixels::. • The output will have the same type as the inputs. This is natural for the ‘min’ and ‘max’ operators, but for other similar operators (for example ‘sum’, or ‘average’) the per-pixel operations will be done in double precision floating point and then stored back in the input type. Therefore, if the input was an integer, C’s internal type conversion will be used. ‘max’ Similar to ‘min’, but the pixels of the output will contain the maximum of the respective pixels in all operands in the stack. ‘num’ Similar to ‘min’, but the pixels of the output will contain the number of the respective non-blank pixels in all input operands. ‘sum’ Similar to ‘min’, but the pixels of the output will contain the sum of the respective pixels in all input operands. ‘mean’ Similar to ‘min’, but the pixels of the output will contain the mean (average) of the respective pixels in all operands in the stack. ‘std’ Similar to ‘min’, but the pixels of the output will contain the standard deviation of the respective pixels in all operands in the stack. ‘median’ Similar to ‘min’, but the pixels of the output will contain the median of the respective pixels in all operands in the stack. ‘filter-mean’ Apply mean filtering (or moving average (https://en.wikipedia.org/wiki/Moving_average)) on the input dataset. During mean filtering, each pixel (data element) is replaced by the mean value of all its surrounding pixels (excluding blank values). The number of surrounding pixels in each dimension (to calculate the mean) is determined through the earlier operands that have been pushed onto the stack prior to the input dataset. The number of necessary operands is determined by the dimensions of the input dataset (first popped operand). The order of the dimensions on the command-line is the order in FITS format. Here is one example: $ astarithmetic 5 4 image.fits filter-mean In this example, each pixel is replaced by the mean of a 5 by 4 box around it. The box is 5 pixels along the first FITS dimension (horizontal when viewed in ds9) and 4 pixels along the second FITS dimension (vertical). Each pixel will be placed in the center of the box that the mean is calculated on. If the given width along a dimension is even, then the center is assumed to be between the pixels (not in the center of a pixel). When the pixel is close to the center, the pixels of the box that fall outside the image are ignored. Therefore, on the edge, less points will be used in calculating the mean. The final effect of mean filtering is to smooth the input image, it is essentially a convolution with a kernel that has identical values for all its pixels (is flat), see *note Convolution process::. ‘filter-median’ Apply median filtering (https://en.wikipedia.org/wiki/Median_filter) on the input dataset. This is very similar to ‘filter-mean’, except that instead of the mean value of the box pixels, the median value is used to replace a pixel value. For more on how to use this operator, please see ‘filter-mean’. The median is less susceptible to outliers compared to the mean. As a result, after median filtering, the pixel values will be more discontinuous than mean filtering. ‘lt’ Less than: If the second popped (or left operand in infix notation, see *note Reverse polish notation::) value is smaller than the first popped operand, then this function will return a value of 1, otherwise it will return a value of 0. If both operands are images, then all the pixels will be compared with their counterparts in the other image. If only one operand is an image, then all the pixels will be compared with the the single value (number) of the other operand. Finally if both are numbers, then the output is also just one number (0 or 1). When the output is not a single number, it will be stored as an ‘unsigned char’ type. ‘le’ Less or equal: similar to ‘lt’ (‘less than’ operator), but returning 1 when the second popped operand is smaller or equal to the first. ‘gt’ Greater than: similar to ‘lt’ (‘less than’ operator), but returning 1 when the second popped operand is greater than the first. ‘ge’ Greater or equal: similar to ‘lt’ (‘less than’ operator), but returning 1 when the second popped operand is larger or equal to the first. ‘eq’ Equality: similar to ‘lt’ (‘less than’ operator), but returning 1 when the two popped operands are equal (to double precision floating point accuracy). ‘ne’ Non-Equality: similar to ‘lt’ (‘less than’ operator), but returning 1 when the two popped operands are _not_ equal (to double precision floating point accuracy). ‘and’ Logical AND: returns 1 if both operands have a non-zero value and 0 if both are zero. Both operands have to be the same kind: either both images or both numbers. ‘or’ Logical OR: returns 1 if either one of the operands is non-zero and 0 only when both operators are zero. Both operands have to be the same kind: either both images or both numbers. ‘not’ Logical NOT: returns 1 when the operand is zero and 0 when the operand is non-zero. The operand can be an image or number, for an image, it is applied to each pixel separately. ‘isblank’ Test for a blank value (see *note Blank pixels::). In essence, this is very similar to the conditional operators: the output is either 1 or 0 (see the ‘less than’ operator above). The difference is that it only needs one operand. Because of the definition of a blank pixel, a blank value is not even equal to itself, so you cannot use the equal operator above to select blank pixels. See the “Blank pixels†box below for more on Blank pixels in Arithmetic. ‘where’ Change the input (pixel) value _where_/if a certain condition holds. The conditional operators above can be used to define the condition. Three operands are required for ‘where’. The input format is demonstrated in this simplified example: $ astarithmetic modify.fits binary.fits if-true.fits where The value of any pixel in ‘modify.fits’ that corresponds to a non-zero pixel of ‘binary.fits’ will be changed to the value of the same pixel in ‘if-true.fits’ (this may also be a number). The 3rd and 2nd popped operands (‘modify.fits’ and ‘binary.fits’ respectively, see *note Reverse polish notation::) have to have the same dimensions/size. ‘if-true.fits’ can be either a number, or have the same dimension/size as the other two. The 2nd popped operand (‘binary.fits’) has to have ‘uint8’ (or ‘unsigned char’ in standard C) type (see *note Numeric data types::). It is treated as a binary dataset (with only two values: zero and non-zero, hence the name ‘binary.fits’ in this example). However, commonly you won’t be dealing with an actual FITS file of a condition/binary image. You will probably define the condition in the same run based on some other reference image and use the conditional and logical operators above to make a true/false (or one/zero) image for you internally. For example the case below: $ astarithmetic in.fits reference.fits 100 gt new.fits where In the example above, any of the ‘in.fits’ pixels that has a value in ‘reference.fits’ greater than ‘100’, will be replaced with the corresponding pixel in ‘new.fits’. Effectively the ‘reference.fits 100 gt’ part created the condition/binary image which was added to the stack (in memory) and later used by ‘where’. The command above is thus equivalent to these two commands: $ astarithmetic reference.fits 100 gt --output=binary.fits $ astarithmetic in.fits binary.fits new.fits where Finally, the input operands are read and used independently, so you can use the same file more than once as any of the operands. When the 1st popped operand to ‘where’ (‘if-true.fits’) is a single number, it may be a NaN value (or any blank value, depending on its type) like the example below (see *note Blank pixels::). When the number is blank, it will be converted to the blank value of the type of the 3rd popped operand (‘in.fits’). Hence, in the example below, all the pixels in ‘reference.fits’ that have a value greater than 100, will become blank in the natural data type of ‘in.fits’ (even though NaN values are only defined for floating point types). $ astarithmetic in.fits reference.fits 100 gt nan where ‘bitand’ Bitwise AND operator: only bits with values of 1 in both popped operands will get the value of 1, the rest will be set to 0. For example (assuming numbers can be written as bit strings on the command-line): ‘00101000 00100010 bitand’ will give ‘00100000’. Note that the bitwise operators only work on integer type datasets. ‘bitor’ Bitwise inclusive OR operator: The bits where at least one of the two popped operands has a 1 value get a value of 1, the others 0. For example (assuming numbers can be written as bit strings on the command-line): ‘00101000 00100010 bitand’ will give ‘00101010’. Note that the bitwise operators only work on integer type datasets. ‘bitxor’ Bitwise exclusive OR operator: A bit will be 1 if it differs between the two popped operands. For example (assuming numbers can be written as bit strings on the command-line): ‘00101000 00100010 bitand’ will give ‘00001010’. Note that the bitwise operators only work on integer type datasets. ‘lshift’ Bitwise left shift operator: shift all the bits of the first operand to the left by a number of times given by the second operand. For example (assuming numbers can be written as bit strings on the command-line): ‘00101000 2 lshift’ will give ‘10100000’. This is equivalent to multiplication by 4. Note that the bitwise operators only work on integer type datasets. ‘rshift’ Bitwise right shift operator: shift all the bits of the first operand to the right by a number of times given by the second operand. For example (assuming numbers can be written as bit strings on the command-line): ‘00101000 2 rshift’ will give ‘00001010’. Note that the bitwise operators only work on integer type datasets. ‘bitnot’ Bitwise not (more formally known as one’s complement) operator: flip all the bits of the popped operand (note that this is the only unary, or single operand, bitwise operator). In other words, any bit with a value of ‘0’ is changed to ‘1’ and vice-versa. For example (assuming numbers can be written as bit strings on the command-line): ‘00101000 bitnot’ will give ‘11010111’. Note that the bitwise operators only work on integer type datasets/numbers. ‘uint8’ Convert the type of the popped operand to 8-bit un-signed integer type (see *note Numeric data types::). The internal conversion of C will be used. ‘int8’ Convert the type of the popped operand to 8-bit signed integer type (see *note Numeric data types::). The internal conversion of C will be used. ‘uint16’ Convert the type of the popped operand to 16-bit un-signed integer type (see *note Numeric data types::). The internal conversion of C will be used. ‘int16’ Convert the type of the popped operand to 16-bit signed integer (see *note Numeric data types::). The internal conversion of C will be used. ‘uint32’ Convert the type of the popped operand to 32-bit un-signed integer type (see *note Numeric data types::). The internal conversion of C will be used. ‘int32’ Convert the type of the popped operand to 32-bit signed integer type (see *note Numeric data types::). The internal conversion of C will be used. ‘uint64’ Convert the type of the popped operand to 64-bit un-signed integer (see *note Numeric data types::). The internal conversion of C will be used. ‘float32’ Convert the type of the popped operand to 32-bit (single precision) floating point (see *note Numeric data types::). The internal conversion of C will be used. ‘float64’ Convert the type of the popped operand to 64-bit (double precision) floating point (see *note Numeric data types::). The internal conversion of C will be used. *Blank pixels in Arithmetic:* Blank pixels in the image (see *note Blank pixels::) will be stored based on the data type. When the input is floating point type, blank values are NaN. One aspect of NaN values is that by definition they will fail on _any_ comparison. Hence both equal and not-equal operators will fail when both their operands are NaN! Therefore, the only way to guarantee selection of blank pixels is through the ‘isblank’ operator explained above. One way you can exploit this property of the NaN value to your advantage is when you want a fully zero-valued image (even over the blank pixels) based on an already existing image (with same size and world coordinate system settings). The following command will produce this for you: $ astarithmetic input.fits nan eq --output=all-zeros.fits Note that on the command-line you can write NaN in any case (for example ‘NaN’, or ‘NAN’ are also acceptable). Reading NaN as a floating point number in Gnuastro isn’t case-sensitive.  File: gnuastro.info, Node: Invoking astarithmetic, Prev: Arithmetic operators, Up: Arithmetic 6.2.3 Invoking Arithmetic ------------------------- Arithmetic will do pixel to pixel arithmetic operations on the individual pixels of input data and/or numbers. For the full list of operators with explanations, please see *note Arithmetic operators::. Any operand that only has a single element (number, or single pixel FITS image) will be read as a number, the rest of the inputs must have the same dimensions. The general template is: $ astarithmetic [OPTION...] ASTRdata1 [ASTRdata2] OPERATOR ... One line examples: ## Calculate (10.32-3.84)^2.7 quietly (will just print 155.329): $ astarithmetic -q 10.32 3.84 - 2.7 pow ## Inverse the input image (1/pixel): $ astarithmetic 1 image.fits / --out=inverse.fits ## Multiply each pixel in image by -1: $ astarithmetic image.fits -1 x --out=negative.fits ## Subtract extension 4 from extension 1 (counting from zero): $ astarithmetic image.fits image.fits - --out=skysub.fits \ --hdu=1 --hdu=4 ## Add two images, then divide them by 2 (2 is read as floating point): $ astarithmetic image1.fits image2.fits + 2f / --out=average.fits ## Use Arithmetic's average operator: $ astarithmetic image1.fits image2.fits average --out=average.fits ## Calculate the median of three images in three separate extensions: $ astarithmetic img1.fits img2.fits img3.fits median \ -h0 -h1 -h2 --out=median.fits If the output is an image, and the ‘--output’ option is not given, automatic output will use the name of the first FITS image encountered to generate an output file name, see *note Automatic output::. Also, output WCS information will be taken from the first input image encountered. When the output is a single number, that number will be printed in the standard output and no output file will be created. Arithmetic’s notation for giving operands to operators is described in *note Reverse polish notation::. To ignore certain pixels, set them as blank, see *note Blank pixels::, for example with the ‘where’ operator (see *note Arithmetic operators::). See *note Common options:: for a review of the options in all Gnuastro programs. Arithmetic just redefines the ‘--hdu’ option as explained below: ‘-h INT/STR’ ‘--hdu INT/STR’ The header data unit of the input FITS images, see *note Input output options::. Unlike most options in Gnuastro (which will ultimately only have one value for this option), Arithmetic allows ‘--hdu’ to be called multiple times and the value of each invocation will be stored separately (for the unlimited number of input images you would like to use). Recall that for other programs this (common) option only takes a single value. So in other programs, if you specify it multiple times on the command-line, only the last value will be used and in the configuration files, it will be ignored if it already has a value. The order of the values to ‘--hdu’ has to be in the same order as input FITS images. Options are first read from the command-line (from left to right), then top-down in each configuration file, see *note Configuration file precedence::. If the number of HDUs is less than the number of input images, Arithmetic will abort and notify you. However, if there are more HDUs than FITS images, there is no problem: they will be used in the given order (every time a FITS image comes up on the stack) and the extra HDUs will be ignored in the end. So there is no problem with having extra HDUs in the configuration files and by default several HDUs with a value of ‘0’ are kept in the system-wide configuration file when you install Gnuastro. ‘-g INT/STR’ ‘--globalhdu INT/STR’ Use the value to this option as the HDU of all input FITS files. This option is very convenient when you have many input files and the dataset of interest is in the same HDU of all the files. When this option is called, any values given to the ‘--hdu’ option (explained above) are ignored and will not be used. Arithmetic accepts two kinds of input: images and numbers. Images are considered to be any of the inputs that is a file name of a recognized type (see *note Arguments::) and has more than one element/pixel. Numbers on the command-line will be read into the smallest type (see *note Numeric data types::) that can store them, so ‘-2’ will be read as a ‘char’ type (which is signed on most systems and can thus keep negative values), ‘2500’ will be read as an ‘unsigned short’ (all positive numbers will be read as unsigned), while ‘3.1415926535897’ will be read as a ‘double’ and ‘3.14’ will be read as a ‘float’. To force a number to be read as float, add a ‘f’ after it, so ‘5f’ will be added to the stack as ‘float’ (see *note Reverse polish notation::). Unless otherwise stated (in *note Arithmetic operators::), the operators can deal with numeric multiple data types (see *note Numeric data types::). For example in “‘a.fits b.fits +’â€, the image types can be ‘long’ and ‘float’. In such cases, C’s internal type conversion will be used. The output type will be set to the higher-ranking type of the two inputs. Unsigned integer types have smaller ranking than their signed counterparts and floating point types have higher ranking than the integer types. So the internal C type conversions done in the example above are equivalent to this piece of C: size_t i; long a[100]; float b[100], out[100]; for(i=0;i<100;++i) out[i]=a[i]+b[i]; Relying on the default C type conversion significantly speeds up the processing and also requires less RAM (when using very large images). Some operators can only work on integer types (of any length, for example bitwise operators) while others only work on floating point types, (currently only the ‘pow’ operator). In such cases, if the operand type(s) are different, an error will be printed. Arithmetic also comes with internal type conversion operators which you can use to convert the data into the appropriate type, see *note Arithmetic operators::. The hyphen (‘-’) can be used both to specify options (see *note Options::) and also to specify a negative number which might be necessary in your arithmetic. In order to enable you to do this, Arithmetic will first parse all the input strings and if the first character after a hyphen is a digit, then that hyphen is temporarily replaced by the vertical tab character which is not commonly used. The arguments are then parsed and these strings will not be specified as an option. Then the given arguments are parsed and any vertical tabs are replaced back with a hyphen so they can be read as negative numbers. Therefore, as long as the names of the files you want to work on, don’t start with a vertical tab followed by a digit, there is no problem. An important consequence of this implementation is that you should not write negative fractions like this: ‘-.3’, instead write them as ‘-0.3’. Without any images, Arithmetic will act like a simple calculator and print the resulting output number on the standard output like the first example above. If you really want such calculator operations on the command-line, AWK (GNU AWK is the most common implementation) is much faster, easier and much more powerful. For example, the numerical one-line example above can be done with the following command. In general AWK is a fantastic tool and GNU AWK has a wonderful manual (). So if you often confront situations like this, or have to work with large text tables/catalogs, be sure to checkout AWK and simplify your life. $ echo "" | awk '{print (10.32-3.84)^2.7}' 155.329  File: gnuastro.info, Node: Convolve, Next: Warp, Prev: Arithmetic, Up: Data manipulation 6.3 Convolve ============ On an image, convolution can be thought of as a process to blur or remove the contrast in an image. If you are already familiar with the concept and just want to run Convolve, you can jump to *note Convolution kernel:: and *note Invoking astconvolve:: and skip the lengthy introduction on the basic definitions and concepts of convolution. There are generally two methods to convolve an image. The first and more intuitive one is in the “spatial domain†or using the actual image pixel values, see *note Spatial domain convolution::. The second method is when we manipulate the “frequency domainâ€, or work on the magnitudes of the different frequencies that constitute the image, see *note Frequency domain and Fourier operations::. Understanding convolution in the spatial domain is more intuitive and thus recommended if you are just starting to learn about convolution. However, getting a good grasp of the frequency domain is a little more involved and needs some concentration and some mathematical proofs. However, its reward is a faster operation and more importantly a very fundamental understanding of this very important operation. Convolution of an image will generally result in blurring the image because it mixes pixel values. In other words, if the image has sharp differences in neighboring pixel values(1), those sharp differences will become smoother. This has very good consequences in detection of signal in noise for example. In an actual observed image, the variation in neighboring pixel values due to noise can be very high. But after convolution, those variations will decrease and we have a better hope in detecting the possible underlying signal. Another case where convolution is extensively used is in mock images and modeling in general, convolution can be used to simulate the effect of the atmosphere or the optical system on the mock profiles that we create, see *note PSF::. Convolution is a very interesting and important topic in any form of signal analysis (including astronomical observations). So we have thoroughly(2) explained the concepts behind it in the following sub-sections. * Menu: * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. ---------- Footnotes ---------- (1) In astronomy, the only major time we confront such sharp borders in signal are cosmic rays. All other sources of signal in an image are already blurred by the atmosphere or the optics of the instrument. (2) A mathematician will certainly consider this explanation is incomplete and inaccurate. However this text is written for an understanding on the operations that are done on a real (not complex, discrete and noisy) astronomical image, not any general form of abstract function  File: gnuastro.info, Node: Spatial domain convolution, Next: Frequency domain and Fourier operations, Prev: Convolve, Up: Convolve 6.3.1 Spatial domain convolution -------------------------------- The pixels in an input image represent different “spatial†positions, therefore when convolution is done only using the actual input pixel values, we name the process as being done in the “Spatial domainâ€. In particular this is in contrast to the “frequency domain†that we will discuss later in *note Frequency domain and Fourier operations::. In the spatial domain (and in realistic situations where the image and the convolution kernel don’t extend to infinity), convolution is the process of changing the value of one pixel to the _weighted_ average of all the pixels in its _neighborhood_. The ‘neighborhood’ of each pixel (how many pixels in which direction) and the ‘weight’ function (how much each neighboring pixel should contribute depending on its position) are given through a second image which is known as a “kernelâ€(1). * Menu: * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. ---------- Footnotes ---------- (1) Also known as filter, here we will use ‘kernel’.  File: gnuastro.info, Node: Convolution process, Next: Edges in the spatial domain, Prev: Spatial domain convolution, Up: Spatial domain convolution 6.3.1.1 Convolution process ........................... In convolution, the kernel specifies the weight and positions of the neighbors of each pixel. To find the convolved value of a pixel, the central pixel of the kernel is placed on that pixel. The values of each overlapping pixel in the kernel and image are multiplied by each other and summed for all the kernel pixels. To have one pixel in the center, the sides of the convolution kernel have to be an odd number. This process effectively mixes the pixel values of each pixel with its neighbors, resulting in a blurred image compared to the sharper input image. Formally, convolution is one kind of linear ‘spatial filtering’ in image processing texts. If we assume that the kernel has $2a+1$ and $2b+1$ pixels on each side, the convolved value of a pixel placed at $x$ and $y$ ($C_{x,y}$) can be calculated from the neighboring pixel values in the input image ($I$) and the kernel ($K$) from $$C_{x,y}=\sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t}.$$ Any pixel coordinate that is outside of the image in the equation above will be considered to be zero. When the kernel is symmetric about its center the blurred image has the same orientation as the original image. However, if the kernel is not symmetric, the image will be affected in the opposite manner, this is a natural consequence of the definition of spatial filtering. In order to avoid this we can rotate the kernel about its center by 180 degrees so the convolved output can have the same original orientation. Technically speaking, only if the kernel is flipped the process is known _Convolution_. If it isn’t it is known as _Correlation_. To be a weighted average, the sum of the weights (the pixels in the kernel) have to be unity. This will have the consequence that the convolved image of an object and un-convolved object will have the same brightness (see *note Flux Brightness and magnitude::), which is natural, because convolution should not eat up the object photons, it only disperses them.  File: gnuastro.info, Node: Edges in the spatial domain, Prev: Convolution process, Up: Spatial domain convolution 6.3.1.2 Edges in the spatial domain ................................... In purely ‘linear’ spatial filtering (convolution), there are problems on the edges of the input image. Here we will explain the problem in the spatial domain. For a discussion of this problem from the frequency domain perspective, see *note Edges in the frequency domain::. The problem originates from the fact that on the edges, in practice(1), the sum of the weights we use on the actual image pixels is not unity. For example, as discussed above, a profile in the center of an image will have the same brightness before and after convolution. However, for partially imaged profile on the edge of the image, the brightness (sum of its pixel fluxes within the image, see *note Flux Brightness and magnitude::) will not be equal, some of the flux is going to be ‘eaten’ by the edges. If you ran ‘$ make check’ on the source files of Gnuastro, you can see the this effect by comparing the ‘convolve_frequency.fits’ with ‘convolve_spatial.fits’ in the ‘./tests/’ directory. In the spatial domain, by default, no assumption will be made about pixels outside of the image or any blank pixels in the image. The problem explained above will also occur on the sides of blank regions (see *note Blank pixels::). The solution to this edge effect problem is only possible in the spatial domain. For pixels near the edge, we have to abandon the assumption that the sum of the kernel pixels is unity during the convolution process(2). So taking $W$ as the sum of the kernel pixels that overlapped with non-blank and in-image pixels, the equation in *note Convolution process:: will become: $$C_{x,y}= { \sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t} \over W}.$$ In this manner, objects which are near the edges of the image or blank pixels will also have the same brightness (within the image) before and after convolution. This correction is applied by default in Convolve when convolving in the spatial domain. To disable it, you can use the ‘--noedgecorrection’ option. In the frequency domain, there is no way to avoid this loss of flux near the edges of the image, see *note Edges in the frequency domain:: for an interpretation from the frequency domain perspective. Note that the edge effect discussed here is different from the one in *note If convolving afterwards::. In making mock images we want to simulate a real observation. In a real observation the images of the galaxies on the sides of the CCD are first blurred by the atmosphere and instrument, then imaged. So light from the parts of a galaxy which are immediately outside the CCD will affect the parts of the galaxy which are covered by the CCD. Therefore in modeling the observation, we have to convolve an image that is larger than the input image by exactly half of the convolution kernel. We can hence conclude that this correction for the edges is only useful when working on actual observed images (where we don’t have any more data on the edges) and not in modeling. ---------- Footnotes ---------- (1) Because we assumed the overlapping pixels outside the input image have a value of zero. (2) ofcourse the sum of the kernel pixels still have to be unity in general.  File: gnuastro.info, Node: Frequency domain and Fourier operations, Next: Spatial vs. Frequency domain, Prev: Spatial domain convolution, Up: Convolve 6.3.2 Frequency domain and Fourier operations --------------------------------------------- Getting a good grip on the frequency domain is usually not an easy job! So we have decided to give the issue a complete review here. Convolution in the frequency domain (see *note Convolution theorem::) heavily relies on the concepts of Fourier transform (*note Fourier transform::) and Fourier series (*note Fourier series::) so we will be investigating these important operations first. It has become something of a cliché for people to say that the Fourier series “is a way to represent a (wave-like) function as the sum of simple sine waves†(from Wikipedia). However, sines themselves are abstract functions, so this statement really adds no extra layer of physical insight. Before jumping head-first into the equations and proofs, we will begin with a historical background to see how the importance of frequencies actually roots in our ancient desire to see everything in terms of circles. A short review of how the complex plane should be interpreted is then given. Having paved the way with these two basics, we define the Fourier series and subsequently the Fourier transform. The final aim is to explain discrete Fourier transform, however some very important concepts need to be solidified first: The Dirac comb, convolution theorem and sampling theorem. So each of these topics are explained in their own separate sub-sub-section before going on to the discrete Fourier transform. Finally we revisit (after *note Edges in the spatial domain::) the problem of convolution on the edges, but this time in the frequency domain. Understanding the sampling theorem and the discrete Fourier transform is very important in order to be able to pull out valuable science from the discrete image pixels. Therefore we have included the mathematical proofs and figures so you can have a clear understanding of these very important concepts. * Menu: * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects.  File: gnuastro.info, Node: Fourier series historical background, Next: Circles and the complex plane, Prev: Frequency domain and Fourier operations, Up: Frequency domain and Fourier operations 6.3.2.1 Fourier series historical background ............................................ Ever since the ancient times, the circle has been (and still is) the simplest shape for abstract comprehension. All you need is a center point and a radius and you are done. All the points on a circle are at a fixed distance from the center. However, the moment you try to connect this elegantly simple and beautiful abstract construct (the circle) with the real world (for example compute its area or its circumference), things become really hard (ideally, impossible) because the irrational number $\pi$ gets involved. The key to understanding the Fourier series (thus the Fourier transform and finally the Discrete Fourier Transform) is our ancient desire to express everything in terms of circles or the most exceptionally simple and elegant abstract human construct. Most people prefer to say the same thing in a more ahistorical manner: to break a function into sines and cosines. As the term “ancient†in the previous sentence implies, Jean-Baptiste Joseph Fourier (1768 – 1830 A.D.) was not the first person to do this. The main reason we know this process by his name today is that he came up with an ingenious method to find the necessary coefficients (radius of) and frequencies (“speed†of rotation on) the circles for any generic (integrable) function. [image src="gnuastro-figures/epicycles.png" alt="Middle ages epicycles along with two demonstrations of breaking a generic function using epicycles." text="../gnuastro-figures//epicycles.png"] Figure 6.1: Epicycles and the Fourier series. Left: A demonstration of Mercury’s epicycles relative to the “center of the world†by Qutb al-Din al-Shirazi (1236 – 1311 A.D.) retrieved from Wikipedia (https://commons.wikimedia.org/wiki/File:Ghotb2.jpg). Middle (https://commons.wikimedia.org/wiki/File:Fourier_series_square_wave_circles_animation.gif) and Right: How adding more epicycles (or terms in the Fourier series) will approximate functions. The right (https://commons.wikimedia.org/wiki/File:Fourier_series_sawtooth_wave_circles_animation.gif) animation is also available. Like most aspects of mathematics, this process of interpreting everything in terms of circles, began for astronomical purposes. When astronomers noticed that the orbit of Mars and other outer planets, did not appear to be a simple circle (as everything should have been in the heavens). At some point during their orbit, the revolution of these planets would become slower, stop, go back a little (in what is known as the retrograde motion) and then continue going forward again. The correction proposed by Ptolemy (90 – 168 A.D.) was the most agreed upon. He put the planets on Epicycles or circles whose center itself rotates on a circle whose center is the earth. Eventually, as observations became more and more precise, it was necessary to add more and more epicycles in order to explain the complex motions of the planets(1). *note Figure 6.1: epicycle.(Left) shows an example depiction of the epicycles of Mercury in the late 13th century. Of course we now know that if they had abdicated the Earth from its throne in the center of the heavens and allowed the Sun to take its place, everything would become much simpler and true. But there wasn’t enough observational evidence for changing the “professional consensus†of the time to this radical view suggested by a small minority(2). So the pre-Galilean astronomers chose to keep Earth in the center and find a correction to the models (while keeping the heavens a purely “circular†order). The main reason we are giving this historical background which might appear off topic is to give historical evidence that while such “approximations†do work and are very useful for pragmatic reasons (like measuring the calendar from the movement of astronomical bodies). They offer no physical insight. The astronomers who were involved with the Ptolemaic world view had to add a huge number of epicycles during the centuries after Ptolemy in order to explain more accurate observations. Finally the death knell of this world-view was Galileo’s observations with his new instrument (the telescope). So the physical insight, which is what Astronomers and Physicists are interested in (as opposed to Mathematicians and Engineers who just like proving and optimizing or calculating!) comes from being creative and not limiting our selves to such approximations. Even when they work. ---------- Footnotes ---------- (1) See the Wikipedia page on “Deferent and epicycle†for a more complete historical review. (2) Aristarchus of Samos (310 – 230 B.C.) appears to be one of the first people to suggest the Sun being in the center of the universe. This approach to science (that the standard model is defined by consensus) and the fact that this consensus might be completely wrong still applies equally well to our models of particle physics and cosmology today.  File: gnuastro.info, Node: Circles and the complex plane, Next: Fourier series, Prev: Fourier series historical background, Up: Frequency domain and Fourier operations 6.3.2.2 Circles and the complex plane ..................................... Before going onto the derivation, it is also useful to review how the complex numbers and their plane relate to the circles we talked about above. The two schematics in the middle and right of *note Figure 6.1: epicycle. show how a 1D function of time can be made using the 2D real and imaginary surface. Seeing the animation in Wikipedia will really help in understanding this important concept. At each point in time, we take the vertical coordinate of the point and use it to find the value of the function at that point in time. *note Figure 6.2: iandtime. shows this relation with the axes marked. Leonhard Euler(1) (1707 – 1783 A.D.) showed that the complex exponential ($e^{iv}$ where $v$ is real) is periodic and can be written as: $e^{iv}=\cos{v}+isin{v}$. Therefore $e^{iv+2\pi}=e^{iv}$. Later, Caspar Wessel (mathematician and cartographer 1745 – 1818 A.D.) showed how complex numbers can be displayed as vectors on a plane. Euler’s identity might seem counter intuitive at first, so we will try to explain it geometrically (for deeper physical insight). On the real-imaginary 2D plane (like the left hand plot in each box of *note Figure 6.2: iandtime.), multiplying a number by $i$ can be interpreted as rotating the point by $90$ degrees (for example the value $3$ on the real axis becomes $3i$ on the imaginary axis). On the other hand, $e\equiv\lim_{n\rightarrow\infty}(1+{1\over n})^n$, therefore, defining $m\equiv nu$, we get: $$e^{u}=\lim_{n\rightarrow\infty}\left(1+{1\over n}\right)^{nu} =\lim_{n\rightarrow\infty}\left(1+{u\over nu}\right)^{nu} =\lim_{m\rightarrow\infty}\left(1+{u\over m}\right)^{m}$$ Taking $u\equiv iv$ the result can be written as a generic complex number (a function of $v$): $$e^{iv}=\lim_{m\rightarrow\infty}\left(1+i{v\over m}\right)^{m}=a(v)+ib(v)$$ For $v=\pi$, a nice geometric animation of going to the limit can be seen on Wikipedia (https://commons.wikimedia.org/wiki/File:ExpIPi.gif). We see that $\lim_{m\rightarrow\infty}a(\pi)=-1$, while $\lim_{m\rightarrow\infty}b(\pi)=0$, which gives the famous $e^{i\pi}=-1$ equation. The final value is the real number $-1$, however the distance of the polygon points traversed as $m\rightarrow\infty$ is half the circumference of a circle or $\pi$, showing how $v$ in the equation above can be interpreted as an angle in units of radians and therefore how $a(v)=cos(v)$ and $b(v)=sin(v)$. Since $e^{iv}$ is periodic (let’s assume with a period of $T$), it is more clear to write it as $v\equiv{2{\pi}n\over T}t$ (where $n$ is an integer), so $e^{iv}=e^{i{2{\pi}n\over T}t}$. The advantage of this notation is that the period ($T$) is clearly visible and the frequency ($2{\pi}n \over T$, in units of 1/cycle) is defined through the integer $n$. In this notation, $t$ is in units of “cycleâ€s. As we see from the examples in *note Figure 6.1: epicycle. and *note Figure 6.2: iandtime, for each constituting frequency, we need a respective ‘magnitude’ or the radius of the circle in order to accurately approximate the desired 1D function. The concepts of “period†and “frequency†are relatively easy to grasp when using temporal units like time because this is how we define them in every-day life. However, in an image (astronomical data), we are dealing with spatial units like distance. Therefore, by one “period†we mean the _distance_ at which the signal is identical and frequency is defined as the inverse of that spatial “periodâ€. The complex circle of *note Figure 6.2: iandtime. can be thought of the Moon rotating about Earth which is rotating around the Sun; so the “Real (signal)†axis shows the Moon’s position as seen by a distant observer on the Sun as time goes by. Because of the scalar (not having any direction or vector) nature of time, *note Figure 6.2: iandtime. is easier to understand in units of time. When thinking about spatial units, mentally replace the “Time (sec)†axis with “Distance (meters)â€. Because length has direction and is a vector, visualizing the rotation of the imaginary circle and the advance along the “Distance (meters)†axis is not as simple as temporal units like time. [image src="gnuastro-figures/iandtime.png" text="../gnuastro-figures//iandtime.eps"] Figure 6.2: Relation between the real (signal), imaginary ($i\equiv\sqrt{-1}$) and time axes at two snapshots of time. ---------- Footnotes ---------- (1) Other forms of this equation were known before Euler. For example in 1707 A.D. (the year of Euler’s birth) Abraham de Moivre (1667 – 1754 A.D.) showed that $(\cos{x}+i\sin{x})^n=\cos(nx)+i\sin(nx)$. In 1714 A.D., Roger Cotes (1682 – 1716 A.D. a colleague of Newton who proofread the second edition of Principia) showed that: $ix=\ln(\cos{x}+i\sin{x})$.  File: gnuastro.info, Node: Fourier series, Next: Fourier transform, Prev: Circles and the complex plane, Up: Frequency domain and Fourier operations 6.3.2.3 Fourier series ...................... In astronomical images, our variable (brightness, or number of photo-electrons, or signal to be more generic) is recorded over the 2D spatial surface of a camera pixel. However to make things easier to understand, here we will assume that the signal is recorded in 1D (assume one row of the 2D image pixels). Also for this section and the next (*note Fourier transform::) we will be talking about the signal before it is digitized or pixelated. Let’s assume that we have the continuous function $f(l)$ which is integrable in the interval $[l_0, l_0+L]$ (always true in practical cases like images). Take $l_0$ as the position of the first pixel in the assumed row of the image and $L$ as the width of the image along that row. The units of $l_0$ and $L$ can be in any spatial units (for example meters) or an angular unit (like radians) multiplied by a fixed distance which is more common. To approximate $f(l)$ over this interval, we need to find a set of frequencies and their corresponding ‘magnitude’s (see *note Circles and the complex plane::). Therefore our aim is to show $f(l)$ as the following sum of periodic functions: $$f(l)=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over L}l} $$ Note that the different frequencies ($2{\pi}n/L$, in units of cycles per meters for example) are not arbitrary. They are all integer multiples of the fundamental frequency of $\omega_0=2\pi/L$. Recall that $L$ was the length of the signal we want to model. Therefore, we see that the smallest possible frequency (or the frequency resolution) in the end, depends on the length we observed the signal or $L$. In the case of each dimension on an image, this is the size of the image in the respective dimension. The frequencies have been defined in this “harmonic†fashion to insure that the final sum is periodic outside of the $[l_0, l_0+L]$ interval too. At this point, you might be thinking that the sky is not periodic with the same period as my camera’s view angle. You are absolutely right! The important thing is that since your camera’s observed region is the only region we are “observing†and will be using, the rest of the sky is irrelevant; so we can safely assume the sky is periodic outside of it. However, this working assumption will haunt us later in *note Edges in the frequency domain::. The frequencies are thus determined by definition. So all we need to do is to find the coefficients ($c_n$), or magnitudes, or radii of the circles for each frequency which is identified with the integer $n$. Fourier’s approach was to multiply both sides with a fixed term: $$f(l)e^{-i{2{\pi}m\over L}l}=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l} $$ where $m>0$(1). We can then integrate both sides over the observation period: $$\int_{l_0}^{l_0+L}f(l)e^{-i{2{\pi}m\over L}l}dl =\int_{l_0}^{l_0+L}\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l}dl=\displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+L}e^{i{2{\pi}(n-m)\over L}l}dl $$ Both $n$ and $m$ are positive integers. Also, we know that a complex exponential is periodic so after one period ($L$) it comes back to its starting point. Therefore $\int_{l_0}^{l_0+L}e^{2{\pi}k/L}dl=0$ for any $k>0$. However, when $k=0$, this integral becomes: $\int_{l_0}^{l_0+T}e^0dt=\int_{l_0}^{l_0+T}dt=T$. Hence since the integral will be zero for all $n{\neq}m$, we get: $$\displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+T}e^{i{2{\pi}(n-m)\over L}l}dl=Lc_m $$ The origin of the axis is fundamentally an arbitrary position. So let’s set it to the start of the image such that $l_0=0$. So we can find the “magnitude†of the frequency $2{\pi}m/L$ within $f(l)$ through the relation: $$c_m={1\over L}\int_{0}^{L}f(l)e^{-i{2{\pi}m\over L}l}dl $$ ---------- Footnotes ---------- (1) We could have assumed $m<0$ and set the exponential to positive, but this is more clear.  File: gnuastro.info, Node: Fourier transform, Next: Dirac delta and comb, Prev: Fourier series, Up: Frequency domain and Fourier operations 6.3.2.4 Fourier transform ......................... In *note Fourier series::, we had to assume that the function is periodic outside of the desired interval with a period of $L$. Therefore, assuming that $L\rightarrow\infty$ will allow us to work with any function. However, with this approximation, the fundamental frequency ($\omega_0$) or the frequency resolution that we discussed in *note Fourier series:: will tend to zero: $\omega_0\rightarrow0$. In the equation to find $c_m$, every $m$ represented a frequency (multiple of $\omega_0$) and the integration on $l$ removes the dependence of the right side of the equation on $l$, making it only a function of $m$ or frequency. Let’s define the following two variables: $$\omega{\equiv}m\omega_0={2{\pi}m\over L}$$ $$F(\omega){\equiv}Lc_m$$ The equation to find the coefficients of each frequency in *note Fourier series:: thus becomes: $$F(\omega)=\int_{-\infty}^{\infty}f(l)e^{-i{\omega}l}dl. $$ The function $F(\omega)$ is thus the _Fourier transform_ of $f(l)$ in the frequency domain. So through this transformation, we can find (analyze) the magnitudes of the constituting frequencies or the value in the frequency space(1) of our spatial input function. The great thing is that we can also do the reverse and later synthesize the input function from its Fourier transform. Let’s do it: with the approximations above, multiply the right side of the definition of the Fourier Series (*note Fourier series::) with $1=L/L=({\omega_0}L)/(2\pi)$: $$f(l)={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}Lc_ne^{{2{\pi}in\over L}l}\omega_0={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}F(\omega)e^{i{\omega}l}\Delta\omega $$ To find the right most side of this equation, we renamed $\omega_0$ as $\Delta\omega$ because it was our resolution, $2{\pi}n/L$ was written as $\omega$ and finally, $Lc_n$ was written as $F(\omega)$ as we defined above. Now, as $L\rightarrow\infty$, $\Delta\omega\rightarrow0$ so we can write: $$f(l)={1\over 2\pi}\int_{-\infty}^{\infty}F(\omega)e^{i{\omega}l}d\omega $$ Together, these two equations provide us with a very powerful set of tools that we can use to process (analyze) and recreate (synthesize) the input signal. Through the first equation, we can break up our input function into its constituent frequencies and analyze it, hence it is also known as _analysis_. Using the second equation, we can synthesize or make the input function from the known frequencies and their magnitudes. Thus it is known as _synthesis_. Here, we symbolize the Fourier transform (analysis) and its inverse (synthesis) of a function $f(l)$ and its Fourier Transform $F(\omega)$ as ${\cal F}[f]$ and ${\cal F}^{-1}[F]$. ---------- Footnotes ---------- (1) As we discussed before, this ‘magnitude’ can be interpreted as the radius of the circle rotating at this frequency in the epicyclic interpretation of the Fourier series, see *note Figure 6.1: epicycle. and *note Figure 6.2: iandtime.  File: gnuastro.info, Node: Dirac delta and comb, Next: Convolution theorem, Prev: Fourier transform, Up: Frequency domain and Fourier operations 6.3.2.5 Dirac delta and comb ............................ The Dirac $\delta$ (delta) function (also known as an impulse) is the way that we convert a continuous function into a discrete one. It is defined to satisfy the following integral: $$\int_{-\infty}^{\infty}\delta(l)dl=1$$ When integrated with another function, it gives that function’s value at $l=0$: $$\int_{-\infty}^{\infty}f(l)\delta(l)dt=f(0)$$ An impulse positioned at another point (say $l_0$) is written as $\delta(l-l_0)$: $$\int_{-\infty}^{\infty}f(l)\delta(l-l_0)dt=f(l_0)$$ The Dirac $\delta$ function also operates similarly if we use summations instead of integrals. The Fourier transform of the delta function is: $${\cal F}[\delta(l)]=\int_{-\infty}^{\infty}\delta(l)e^{-i{\omega}l}dl=e^{-i{\omega}0}=1$$ $${\cal F}[\delta(l-l_0)]=\int_{-\infty}^{\infty}\delta(l-l_0)e^{-i{\omega}l}dl=e^{-i{\omega}l_0}$$ From the definition of the Dirac $\delta$ we can also define a Dirac comb (${\rm III}_P$) or an impulse train with infinite impulses separated by $P$: $${\rm III}_P(l)\equiv\displaystyle\sum_{k=-\infty}^{\infty}\delta(l-kP) $$ $P$ is chosen to represent “pixel width†later in *note Sampling theorem::. Therefore the Dirac comb is periodic with a period of $P$. We have intentionally used a different name for the period of the Dirac comb compared to the input signal’s length of observation that we showed with $L$ in *note Fourier series::. This difference is highlighted here to avoid confusion later when these two periods are needed together in *note Discrete Fourier transform::. The Fourier transform of the Dirac comb will be necessary in *note Sampling theorem::, so let’s derive it. By its definition, it is periodic, with a period of $P$, so the Fourier coefficients of its Fourier Series (*note Fourier series::) can be calculated within one period: $${\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over P}l}$$ We can now find the $c_n$ from *note Fourier series::: $$c_n={1\over P}\int_{-P/2}^{P/2}\delta(l)e^{-i{2{\pi}n\over P}l} ={1\over P}\quad\quad \rightarrow \quad\quad {\rm III}_P={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}e^{i{2{\pi}n\over P}l} $$ So we can write the Fourier transform of the Dirac comb as: $${\cal F}[{\rm III}_P]=\int_{-\infty}^{\infty}{\rm III}_Pe^{-i{\omega}l}dl ={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}e^{-i(\omega-{2{\pi}n\over P})l}dl={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\delta\left(\omega-{2{\pi}n\over P}\right) $$ In the last step, we used the fact that the complex exponential is a periodic function, that $n$ is an integer and that as we defined in *note Fourier transform::, $\omega{\equiv}m\omega_0$, where $m$ was an integer. The integral will be zero for any $\omega$ that is not equal to $2{\pi}n/P$, a more complete explanation can be seen in *note Fourier series::. Therefore, while in the spatial domain the impulses had spacing of $P$ (meters for example), in the frequency space, the spacing between the different impulses are $2\pi/P$ cycles per meters.  File: gnuastro.info, Node: Convolution theorem, Next: Sampling theorem, Prev: Dirac delta and comb, Up: Frequency domain and Fourier operations 6.3.2.6 Convolution theorem ........................... The convolution (shown with the $\ast$ operator) of the two functions $f(l)$ and $h(l)$ is defined as: $$c(l)\equiv[f{\ast}h](l)=\int_{-\infty}^{\infty}f(\tau)h(l-\tau)d\tau $$ See *note Convolution process:: for a more detailed physical (pixel based) interpretation of this definition. The Fourier transform of convolution ($C(\omega)$) can be written as: $$ C(\omega)=\int_{-\infty}^{\infty}[f{\ast}h](l)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}f(\tau)\left[\int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl\right]d\tau $$ To solve the inner integral, let’s define $s{\equiv}l-\tau$, so that $ds=dl$ and $l=s+\tau$ then the inner integral becomes: $$\int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}h(s)e^{-i{\omega}(s+\tau)}ds=e^{-i{\omega}\tau}\int_{-\infty}^{\infty}h(s)e^{-i{\omega}s}ds=H(\omega)e^{-i{\omega}\tau} $$ where $H(\omega)$ is the Fourier transform of $h(l)$. Substituting this result for the inner integral above, we get: $$C(\omega)=H(\omega)\int_{-\infty}^{\infty}f(\tau)e^{-i{\omega}\tau}d\tau=H(\omega)F(\omega)=F(\omega)H(\omega) $$ where $F(\omega)$ is the Fourier transform of $f(l)$. So multiplying the Fourier transform of two functions individually, we get the Fourier transform of their convolution. The convolution theorem also proves a relation between the convolutions in the frequency space. Let’s define: $$D(\omega){\equiv}F(\omega){\ast}H(\omega)$$ Applying the inverse Fourier Transform or synthesis equation (*note Fourier transform::) to both sides and following the same steps above, we get: $$d(l)=f(l)h(l)$$ Where $d(l)$ is the inverse Fourier transform of $D(\omega)$. We can therefore re-write the two equations above formally as the convolution theorem: $$ {\cal F}[f{\ast}h]={\cal F}[f]{\cal F}[h] $$ $$ {\cal F}[fh]={\cal F}[f]\ast{\cal F}[h] $$ Besides its usefulness in blurring an image by convolving it with a given kernel, the convolution theorem also enables us to do another very useful operation in data analysis: to match the blur (or PSF) between two images taken with different telescopes/cameras or under different atmospheric conditions. This process is also known as de-convolution. Let’s take $f(l)$ as the image with a narrower PSF (less blurry) and $c(l)$ as the image with a wider PSF which appears more blurred. Also let’s take $h(l)$ to represent the kernel that should be convolved with the sharper image to create the more blurry image. Above, we proved the relation between these three images through the convolution theorem. But there, we assumed that $f(l)$ and $h(l)$ are known (given) and the convolved image is desired. In de-convolution, we have $f(l)$ –the sharper image– and $f*h(l)$ –the more blurry image– and we want to find the kernel $h(l)$. The solution is a direct result of the convolution theorem: $$ {\cal F}[h]={{\cal F}[f{\ast}h]\over {\cal F}[f]} \quad\quad {\rm or} \quad\quad h(l)={\cal F}^{-1}\left[{{\cal F}[f{\ast}h]\over {\cal F}[f]}\right] $$ While this works really nice, it has two problems: • If ${\cal F}[f]$ has any zero values, then the inverse Fourier transform will not be a number! • If there is significant noise in the image, then the high frequencies of the noise are going to significantly reduce the quality of the final result. A standard solution to both these problems is the Weiner de-convolution algorithm(1). ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: Sampling theorem, Next: Discrete Fourier transform, Prev: Convolution theorem, Up: Frequency domain and Fourier operations 6.3.2.7 Sampling theorem ........................ Our mathematical functions are continuous, however, our data collecting and measuring tools are discrete. Here we want to give a mathematical formulation for digitizing the continuous mathematical functions so that later, we can retrieve the continuous function from the digitized recorded input. Assuming that we have a continuous function $f(l)$, then we can define $f_s(l)$ as the ‘sampled’ $f(l)$ through the Dirac comb (see *note Dirac delta and comb::): $$f_s(l)=f(l){\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}f(l)\delta(l-nP) $$ The discrete data-element $f_k$ (for example, a pixel in an image), where $k$ is an integer, can thus be represented as: $$f_k=\int_{-\infty}^{\infty}f_s(l)dl=\int_{-\infty}^{\infty}f(l)\delta(l-kP)dt=f(kP)$$ Note that in practice, our discrete data points are not found in this fashion. Each detector pixel (in an image for example) has an area and averages the signal it receives over that area, not a mathematical point as the Dirac $\delta$ function defines. However, as long as the variation in the signal over one detector pixel is not significant, this can be a good approximation. Having put this issue to the side, we can now try to find the relation between the Fourier transforms of the un-sampled $f(l)$ and the sampled $f_s(l)$. For a more clear notation, let’s define: $$F_s(\omega)\equiv{\cal F}[f_s]$$ $$D(\omega)\equiv{\cal F}[{\rm III}_P]$$ Then using the Convolution theorem (see *note Convolution theorem::), $F_s(\omega)$ can be written as: $$F_s(\omega)={\cal F}[f(l){\rm III}_P]=F(\omega){\ast}D(\omega)$$ Finally, from the definition of convolution and the Fourier transform of the Dirac comb (see *note Dirac delta and comb::), we get: $$\eqalign{ F_s(\omega) &= \int_{-\infty}^{\infty}F(\omega)D(\omega-\mu)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}F(\omega)\delta\left(\omega-\mu-{2{\pi}n\over P}\right)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}F\left( \omega-{2{\pi}n\over P}\right).\cr } $$ $F(\omega)$ was only a simple function, see *note Figure 6.3: samplingfreq.(left). However, from the sampled Fourier transform function we see that $F_s(\omega)$ is the superposition of infinite copies of $F(\omega)$ that have been shifted, see *note Figure 6.3: samplingfreq.(right). From the equation, it is clear that the shift in each copy is $2\pi/P$. [image src="gnuastro-figures/samplingfreq.png" text="../gnuastro-figures//samplingfreq.eps"] Figure 6.3: Sampling causes infinite repetition in the frequency domain. FT is an abbreviation for ‘Fourier transform’. $\omega_m$ represents the maximum frequency present in the input. $F(\omega)$ is only symmetric on both sides of 0 when the input is real (not complex). In general $F(\omega)$ is complex and thus cannot be simply plotted like this. Here we have assumed a real Gaussian $f(t)$ which has produced a Gaussian $F(\omega)$. The input $f(l)$ can have any distribution of frequencies in it. In the example of *note Figure 6.3: samplingfreq.(left), the input consisted of a range of frequencies equal to $\Delta\omega=2\omega_m$. Fortunately as *note Figure 6.3: samplingfreq.(right) shows, the assumed pixel size ($P$) we used to sample this hypothetical function was such that $2\pi/P>\Delta\omega$. The consequence is that each copy of $F(\omega)$ has become completely separate from the surrounding copies. Such a digitized (sampled) data set is thus called _over-sampled_. When $2\pi/P=\Delta\omega$, $P$ is just small enough to finely separate even the largest frequencies in the input signal and thus it is known as _critically-sampled_. Finally if $2\pi/P<\Delta\omega$ we are dealing with an _under-sampled_ data set. In an under-sampled data set, the separate copies of $F(\omega)$ are going to overlap and this will deprive us of recovering high constituent frequencies of $f(l)$. The effects of under-sampling in an image with high rates of change (for example a brick wall imaged from a distance) can clearly be visually seen and is known as _aliasing_. When the input $f(l)$ is composed of a finite range of frequencies, $f(l)$ is known as a _band-limited_ function. The example in *note Figure 6.3: samplingfreq.(left) was a nice demonstration of such a case: for all $\omega<-\omega_m$ or $\omega>\omega_m$, we have $F(\omega)=0$. Therefore, when the input function is band-limited and our detector’s pixels are placed such that we have critically (or over-) sampled it, then we can exactly reproduce the continuous $f(l)$ from the discrete or digitized samples. To do that, we just have to isolate one copy of $F(\omega)$ from the infinite copies and take its inverse Fourier transform. This ability to exactly reproduce the continuous input from the sampled or digitized data leads us to the _sampling theorem_ which connects the inherent property of the continuous signal (its maximum frequency) to that of the detector (the spacing between its pixels). The sampling theorem states that the full (continuous) signal can be recovered when the pixel size ($P$) and the maximum constituent frequency in the signal ($\omega_m$) have the following relation(1): $${2\pi\over P}>2\omega_m$$ This relation was first formulated by Harry Nyquist (1889 – 1976 A.D.) in 1928 and formally proved in 1949 by Claude E. Shannon (1916 – 2001 A.D.) in what is now known as the Nyquist-Shannon sampling theorem. In signal processing, the signal is produced (synthesized) by a transmitter and is received and de-coded (analyzed) by a receiver. Therefore producing a band-limited signal is necessary. In astronomy, we do not produce the shapes of our targets, we are only observers. Galaxies can have any shape and size, therefore ideally, our signal is not band-limited. However, since we are always confined to observing through an aperture, the aperture will cause a point source (for which $\omega_m=\infty$) to be spread over several pixels. This spread is quantitatively known as the point spread function or PSF. This spread does blur the image which is undesirable; however, for this analysis it produces the positive outcome that there will be a finite $\omega_m$. Though we should caution that any detector will have noise which will add lots of very high frequency (ideally infinite) changes between the pixels. However, the coefficients of those noise frequencies are usually exceedingly small. ---------- Footnotes ---------- (1) This equation is also shown in some places without the $2\pi$. Whether $2\pi$ is included or not depends on how you define the frequency  File: gnuastro.info, Node: Discrete Fourier transform, Next: Fourier operations in two dimensions, Prev: Sampling theorem, Up: Frequency domain and Fourier operations 6.3.2.8 Discrete Fourier transform .................................. As we have stated several times so far, the input image is a digitized, pixelated or discrete array of values ($f_s(l)$, see *note Sampling theorem::). The input is not a continuous function. Also, all our numerical calculations can only be done on a sampled, or discrete Fourier transform. Note that $F_s(\omega)$ is not discrete, it is continuous. One way would be to find the analytic $F_s(\omega)$, then sample it at any desired “freq-pixelâ€(1) spacing. However, this process would involve two steps of operations and computers in particular are not too good at analytic operations for the first step. So here, we will derive a method to directly find the ‘freq-pixel’ated $F_s(\omega)$ from the pixelated $f_s(l)$. Let’s start with the definition of the Fourier transform (see *note Fourier transform::): $$F_s(\omega)=\int_{-\infty}^{\infty}f_s(l)e^{-i{\omega}l}dl $$ From the definition of $f_s(\omega)$ (using $x$ instead of $n$) we get: $$\eqalign{ F_s(\omega) &= \displaystyle\sum_{x=-\infty}^{\infty} \int_{-\infty}^{\infty}f(l)\delta(l-xP)e^{-i{\omega}l}dl \cr &= \displaystyle\sum_{x=-\infty}^{\infty} f_xe^{-i{\omega}xP} } $$ Where $f_x$ is the value of $f(l)$ on the point $x$ or the value of the $x$th pixel. As shown in *note Sampling theorem:: this function is infinitely periodic with a period of $2\pi/P$. So all we need is the values within one period: $0<\omega<2\pi/P$, see *note Figure 6.3: samplingfreq. We want $X$ samples within this interval, so the frequency difference between each frequency sample or freq-pixel is $1/XP$. Hence we will evaluate the equation above on the points at: $$\omega={u\over XP} \quad\quad u = 0, 1, 2, ..., X-1$$ Therefore the value of the freq-pixel $u$ in the frequency domain is: $$F_u=\displaystyle\sum_{x=0}^{X-1} f_xe^{-i{ux\over X}} $$ Therefore, we see that for each freq-pixel in the frequency domain, we are going to need all the pixels in the spatial domain(2). If the input (spatial) pixel row is also $X$ pixels wide, then we can exactly recover the $x$th pixel with the following summation: $$f_x={1\over X}\displaystyle\sum_{u=0}^{X-1} F_ue^{i{ux\over X}} $$ When the input pixel row (we are still only working on 1D data) has $X$ pixels, then it is $L=XP$ spatial units wide. $L$, or the length of the input data was defined in *note Fourier series:: and $P$ or the space between the pixels in the input was defined in *note Dirac delta and comb::. As we saw in *note Sampling theorem::, the input (spatial) pixel spacing ($P$) specifies the range of frequencies that can be studied and in *note Fourier series:: we saw that the length of the (spatial) input, ($L$) determines the resolution (or size of the freq-pixels) in our discrete Fourier transformed image. Both result from the fact that the frequency domain is the inverse of the spatial domain. ---------- Footnotes ---------- (1) We are using the made-up word “freq-pixel†so they are not confused with spatial domain “pixelsâ€. (2) So even if one pixel is a blank pixel (see *note Blank pixels::), all the pixels in the frequency domain will also be blank.  File: gnuastro.info, Node: Fourier operations in two dimensions, Next: Edges in the frequency domain, Prev: Discrete Fourier transform, Up: Frequency domain and Fourier operations 6.3.2.9 Fourier operations in two dimensions ............................................ Once all the relations in the previous sections have been clearly understood in one dimension, it is very easy to generalize them to two or even more dimensions since each dimension is by definition independent. Previously we defined $l$ as the continuous variable in 1D and the inverse of the period in its direction to be $\omega$. Let’s show the second spatial direction with $m$ the the inverse of the period in the second dimension with $\nu$. The Fourier transform in 2D (see *note Fourier transform::) can be written as: $$F(\omega, \nu)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} f(l, m)e^{-i({\omega}l+{\nu}m)}dl$$ $$f(l, m)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} F(\omega, \nu)e^{i({\omega}l+{\nu}m)}dl$$ The 2D Dirac $\delta(l,m)$ is non-zero only when $l=m=0$. The 2D Dirac comb (or Dirac brush! See *note Dirac delta and comb::) can be written in units of the 2D Dirac $\delta$. For most image detectors, the sides of a pixel are equal in both dimensions. So $P$ remains unchanged, if a specific device is used which has non-square pixels, then for each dimension a different value should be used. $${\rm III}_P(l, m)\equiv\displaystyle\sum_{j=-\infty}^{\infty} \displaystyle\sum_{k=-\infty}^{\infty} \delta(l-jP, m-kP) $$ The Two dimensional Sampling theorem (see *note Sampling theorem::) is thus very easily derived as before since the frequencies in each dimension are independent. Let’s take $\nu_m$ as the maximum frequency along the second dimension. Therefore the two dimensional sampling theorem says that a 2D band-limited function can be recovered when the following conditions hold(1): $${2\pi\over P} > 2\omega_m \quad\quad\quad {\rm and} \quad\quad\quad {2\pi\over P} > 2\nu_m$$ Finally, let’s represent the pixel counter on the second dimension in the spatial and frequency domains with $y$ and $v$ respectively. Also let’s assume that the input image has $Y$ pixels on the second dimension. Then the two dimensional discrete Fourier transform and its inverse (see *note Discrete Fourier transform::) can be written as: $$F_{u,v}=\displaystyle\sum_{x=0}^{X-1}\displaystyle\sum_{y=0}^{Y-1} f_{x,y}e^{-i({ux\over X}+{vy\over Y})} $$ $$f_{x,y}={1\over XY}\displaystyle\sum_{u=0}^{X-1}\displaystyle\sum_{v=0}^{Y-1} F_{u,v}e^{i({ux\over X}+{vy\over Y})} $$ ---------- Footnotes ---------- (1) If the pixels are not a square, then each dimension has to use the respective pixel size, but since most detectors have square pixels, we assume so here too  File: gnuastro.info, Node: Edges in the frequency domain, Prev: Fourier operations in two dimensions, Up: Frequency domain and Fourier operations 6.3.2.10 Edges in the frequency domain ...................................... With a good grasp of the frequency domain, we can revisit the problem of convolution on the image edges, see *note Edges in the spatial domain::. When we apply the convolution theorem (see *note Convolution theorem::) to convolve an image, we first take the discrete Fourier transforms (DFT, *note Discrete Fourier transform::) of both the input image and the kernel, then we multiply them with each other and then take the inverse DFT to construct the convolved image. Of course, in order to multiply them with each other in the frequency domain, the two images have to be the same size, so let’s assume that we pad the kernel (it is usually smaller than the input image) with zero valued pixels in both dimensions so it becomes the same size as the input image before the DFT. Having multiplied the two DFTs, we now apply the inverse DFT which is where the problem is usually created. If the DFT of the kernel only had values of 1 (unrealistic condition!) then there would be no problem and the inverse DFT of the multiplication would be identical with the input. However in real situations, the kernel’s DFT has a maximum of 1 (because the sum of the kernel has to be one, see *note Convolution process::) and decreases something like the hypothetical profile of *note Figure 6.3: samplingfreq. So when multiplied with the input image’s DFT, the coefficients or magnitudes (see *note Circles and the complex plane::) of the smallest frequency (or the sum of the input image pixels) remains unchanged, while the magnitudes of the higher frequencies are significantly reduced. As we saw in *note Sampling theorem::, the Fourier transform of a discrete input will be infinitely repeated. In the final inverse DFT step, the input is in the frequency domain (the multiplied DFT of the input image and the kernel DFT). So the result (our output convolved image) will be infinitely repeated in the spatial domain. In order to accurately reconstruct the input image, we need all the frequencies with the correct magnitudes. However, when the magnitudes of higher frequencies are decreased, longer periods (shorter frequencies) will dominate in the reconstructed pixel values. Therefore, when constructing a pixel on the edge of the image, the newly empowered longer periods will look beyond the input image edges and will find the repeated input image there. So if you convolve an image in this fashion using the convolution theorem, when a bright object exists on one edge of the image, its blurred wings will be present on the other side of the convolved image. This is often termed as circular convolution or cyclic convolution. So, as long as we are dealing with convolution in the frequency domain, there is nothing we can do about the image edges. The least we can do is to eliminate the ghosts of the other side of the image. So, we add zero valued pixels to both the input image and the kernel in both dimensions so the image that will be convolved has a size equal to the sum of both images in each dimension. Of course, the effect of this zero-padding is that the sides of the output convolved image will become dark. To put it another way, the edges are going to drain the flux from nearby objects. But at least it is consistent across all the edges of the image and is predictable. In Convolve, you can see the padded images when inspecting the frequency domain convolution steps with the ‘--viewfreqsteps’ option.  File: gnuastro.info, Node: Spatial vs. Frequency domain, Next: Convolution kernel, Prev: Frequency domain and Fourier operations, Up: Convolve 6.3.3 Spatial vs. Frequency domain ---------------------------------- With the discussions above it might not be clear when to choose the spatial domain and when to choose the frequency domain. Here we will try to list the benefits of each. The spatial domain, • Can correct for the edge effects of convolution, see *note Edges in the spatial domain::. • Can operate on blank pixels. • Can be faster than frequency domain when the kernel is small (in terms of the number of pixels on the sides). The frequency domain, • Will be much faster when the image and kernel are both large. As a general rule of thumb, when working on an image of modeled profiles use the frequency domain and when working on an image of real (observed) objects use the spatial domain (corrected for the edges). The reason is that if you apply a frequency domain convolution to a real image, you are going to loose information on the edges and generally you don’t want large kernels. But when you have made the profiles in the image yourself, you can just make a larger input image and crop the central parts to completely remove the edge effect, see *note If convolving afterwards::. Also due to oversampling, both the kernels and the images can become very large and the speed boost of frequency domain convolution will significantly improve the processing time, see *note Oversampling::.  File: gnuastro.info, Node: Convolution kernel, Next: Invoking astconvolve, Prev: Spatial vs. Frequency domain, Up: Convolve 6.3.4 Convolution kernel ------------------------ All the programs that need convolution will need to be given a convolution kernel file and extension. In most cases (other than Convolve, see *note Convolve::) the kernel file name is optional. However, the extension is necessary and must be specified either on the command-line or at least one of the configuration files (see *note Configuration files::). Within Gnuastro, there are two ways to create a kernel image: • MakeProfiles: You can use MakeProfiles to create a parametric (based on a radial function) kernel, see *note MakeProfiles::. By default MakeProfiles will make the Gaussian and Moffat profiles in a separate file so you can feed it into any of the programs. • ConvertType: You can write your own desired kernel into a text file table and convert it to a FITS file with ConvertType, see *note ConvertType::. Just be careful that the kernel has to have an odd number of pixels along its two axes, see *note Convolution process::. All the programs that do convolution will normalize the kernel internally, so if you choose this option, you don’t have to worry about normalizing the kernel. Only within Convolve, there is an option to disable normalization, see *note Invoking astconvolve::. The two options to specify a kernel file name and its extension are shown below. These are common between all the programs that will do convolution. ‘-k STR’ ‘--kernel=STR’ The convolution kernel file name. The ‘BITPIX’ (data type) value of this file can be any standard type and it does not necessarily have to be normalized. Several operations will be done on the kernel image prior to the program’s processing: • It will be converted to floating point type. • All blank pixels (see *note Blank pixels::) will be set to zero. • It will be normalized so the sum of its pixels equal unity. • It will be flipped so the convolved image has the same orientation. This is only relevant if the kernel is not circular. See *note Convolution process::. ‘-U STR’ ‘--khdu=STR’ The convolution kernel HDU. Although the kernel file name is optional, before running any of the programs, they need to have a value for ‘--khdu’ even if the default kernel is to be used. So be sure to keep its value in at least one of the configuration files (see *note Configuration files::). By default, the system configuration file has a value.  File: gnuastro.info, Node: Invoking astconvolve, Prev: Convolution kernel, Up: Convolve 6.3.5 Invoking Convolve ----------------------- Convolve an input image with a known kernel or make the kernel necessary to match two PSFs. The general template for Convolve is: $ astconvolve [OPTION...] ASTRdata One line examples: ## Convolve mockimg.fits with psf.fits: $ astconvolve --kernel=psf.fits mockimg.fits ## Convolve in the spatial domain: $ astconvolve observedimg.fits --kernel=psf.fits --domain=spatial ## Find the kernel to match sharper and blurry PSF images: $ astconvolve --kernel=sharperimage.fits --makekernel=10 \ blurryimage.fits The only argument accepted by Convolve is an input image file. Some of the options are the same between Convolve and some other Gnuastro programs. Therefore, to avoid repetition, they will not be repeated here. For the full list of options shared by all Gnuastro programs, please see *note Common options::. In particular, in the spatial domain convolve uses Gnuastro’s tessellation, see *note Tessellation:: and the common options related to that in *note Processing options::. Here we will only explain the options particular to Convolve. Run Convolve with ‘--help’ in order to see the full list of options Convolve accepts, irrespective of where they are explained in this book. ‘--nokernelflip’ Do not flip the kernel after reading it the spatial domain convolution. This can be useful if the flipping has already been applied to the kernel. ‘--nokernelnorm’ Do not normalize the kernel after reading it, such that the sum of its pixels is unity. ‘-d STR’ ‘--domain=STR’ The domain to use for the convolution. The acceptable values are ‘‘spatial’’ and ‘‘frequency’’, corresponding to the respective domain. For large images, the frequency domain process will be more efficient than convolving in the spatial domain. However, the edges of the image will loose some flux (see *note Edges in the spatial domain::) and the image must not contain any blank pixels, see *note Spatial vs. Frequency domain::. ‘--checkfreqsteps’ With this option a file with the initial name of the output file will be created that is suffixed with ‘_freqsteps.fits’, all the steps done to arrive at the final convolved image are saved as extensions in this file. The extensions in order are: 1. The padded input image. In frequency domain convolution the two images (input and convolved) have to be the same size and both should be padded by zeros. 2. The padded kernel, similar to the above. 3. The Fourier spectrum of the forward Fourier transform of the input image. Note that the Fourier transform is a complex operation (and not view able in one image!) So we either have to show the ‘Fourier spectrum’ or the ‘Phase angle’. For the complex number $a+ib$, the Fourier spectrum is defined as $\sqrt{a^2+b^2}$ while the phase angle is defined as $\arctan(b/a)$. 4. The Fourier spectrum of the forward Fourier transform of the kernel image. 5. The Fourier spectrum of the multiplied (through complex arithmetic) transformed images. 6. The inverse Fourier transform of the multiplied image. If you open it, you will see that the convolved image is now in the center, not on one side of the image as it started with (in the padded image of the first extension). If you are working on a mock image which originally had pixels of precisely 0.0, you will notice that in those parts that your convolved profile(s) did not convert, the values are now $\sim10^{-18}$, this is due to floating-point round off errors. Therefore in the final step (when cropping the central parts of the image), we also remove any pixel with a value less than $10^{-17}$. ‘--noedgecorrection’ Do not correct the edge effect in spatial domain convolution. For a full discussion, please see *note Edges in the spatial domain::. ‘-m INT’ ‘--makekernel=INT’ (‘=INT’) If this option is called, Convolve will do de-convolution (see *note Convolution theorem::). The image specified by the ‘--kernel’ option is assumed to be the sharper (less blurry) image and the input image is assumed to be the more blurry image. The value given to this option will be used as the maximum radius of the kernel. Any pixel in the final kernel that is larger than this distance from the center will be set to zero. The two images must have the same size. Noise has large frequencies which can make the result less reliable for the higher frequencies of the final result. So all the frequencies which have a spectrum smaller than the value given to the ‘minsharpspec’ option in the sharper input image are set to zero and not divided. This will cause the wings of the final kernel to be flatter than they would ideally be which will make the convolved image result unreliable if it is too high. Some notes to take into account for a good result: • Choose a bright (unsaturated) star and use a region box (with Crop for example, see *note Crop::) that is sufficiently above the noise. • Use Warp (see *note Warp::) to warp the pixel grid so the star’s center is exactly on the center of the central pixel in the cropped image. This will certainly slightly degrade the result, however, it is necessary. If there are multiple good stars, you can shift all of them, then normalize them (so the sum of each star’s pixels is one) and then take their average to decrease this effect. • The shifting might move the center of the star by one pixel in any direction, so crop the central pixel of the warped image to have a clean image for the de-convolution. ‘-c’ ‘--minsharpspec’ (‘=FLT’) The minimum frequency spectrum (or coefficient, or pixel value in the frequency domain image) to use in deconvolution, see the explanations under the ‘--makekernel’ option for more information.  File: gnuastro.info, Node: Warp, Prev: Convolve, Up: Data manipulation 6.4 Warp ======== Image warping is the process of mapping the pixels of one image onto a new pixel grid. This process is sometimes known as transformation, however following the discussion of Heckbert 1989(1) we will not be using that term because it can be confused with only pixel value or flux transformations. Here we specifically mean the pixel grid transformation which is better conveyed with ‘warp’. Image wrapping is a very important step in astronomy, both in observational data analysis and in simulating modeled images. In modeling, warping an image is necessary when we want to apply grid transformations to the initial models, for example in simulating gravitational lensing (Radial warpings are not yet included in Warp). Observational reasons for warping an image are listed below: • *Noise:* Most scientifically interesting targets are inherently faint (have a very low Signal to noise ratio). Therefore one short exposure is not enough to detect such objects that are drowned deeply in the noise. We need multiple exposures so we can add them together and increase the objects’ signal to noise ratio. Keeping the telescope fixed on one field of the sky is practically impossible. Therefore very deep observations have to put into the same grid before adding them. • *Resolution:* If we have multiple images of one patch of the sky (hopefully at multiple orientations) we can warp them to the same grid. The multiple orientations will allow us to ‘guess’ the values of pixels on an output pixel grid that has smaller pixel sizes and thus increase the resolution of the output. This process of merging multiple observations is known as Mosaicing. • *Cosmic rays:* Cosmic rays can randomly fall on any part of an image. If they collide vertically with the camera, they are going to create a very sharp and bright spot that in most cases can be separated easily(2). However, depending on the depth of the camera pixels, and the angle that a cosmic rays collides with it, it can cover a line-like larger area on the CCD which makes the detection using their sharp edges very hard and error prone. One of the best methods to remove cosmic rays is to compare multiple images of the same field. To do that, we need all the images to be on the same pixel grid. • *Optical distortion:* (Not yet included in Warp) In wide field images, the optical distortion that occurs on the outer parts of the focal plane will make accurate comparison of the objects at various locations impossible. It is therefore necessary to warp the image and correct for those distortions prior to the analysis. • *Detector not on focal plane:* In some cases (like the Hubble Space Telescope ACS and WFC3 cameras), the CCD might be tilted compared to the focal plane, therefore the recorded CCD pixels have to be projected onto the focal plane before further analysis. * Menu: * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astwarp:: Arguments and options for Warp. ---------- Footnotes ---------- (1) Paul S. Heckbert. 1989. _Fundamentals of Texture mapping and Image Warping_, Master’s thesis at University of California, Berkeley. (2) All astronomical targets are blurred with the PSF, see *note PSF::, however a cosmic ray is not and so it is very sharp (it suddenly stops at one pixel).  File: gnuastro.info, Node: Warping basics, Next: Merging multiple warpings, Prev: Warp, Up: Warp 6.4.1 Warping basics -------------------- Let’s take $\left[\matrix{u&v}\right]$ as the coordinates of a point in the input image and $\left[\matrix{x&y}\right]$ as the coordinates of that same point in the output image(1). The simplest form of coordinate transformation (or warping) is the scaling of the coordinates, let’s assume we want to scale the first axis by $M$ and the second by $N$, the output coordinates of that point can be calculated by $$\left[\matrix{x\cr y}\right]= \left[\matrix{Mu\cr Nv}\right]= \left[\matrix{M&0\cr0&N}\right]\left[\matrix{u\cr v}\right]$$ Note that these are matrix multiplications. We thus see that we can represent any such grid warping as a matrix. Another thing we can do with this $2\times2$ matrix is to rotate the output coordinate around the common center of both coordinates. If the output is rotated anticlockwise by $\theta$ degrees from the positive (to the right) horizontal axis, then the warping matrix should become: $$\left[\matrix{x\cr y}\right]= \left[\matrix{ucos\theta-vsin\theta\cr usin\theta+vcos\theta}\right]= \left[\matrix{cos\theta&-sin\theta\cr sin\theta&cos\theta}\right] \left[\matrix{u\cr v}\right] $$ We can also flip the coordinates around the first axis, the second axis and the coordinate center with the following three matrices respectively: $$\left[\matrix{1&0\cr0&-1}\right]\quad\quad \left[\matrix{-1&0\cr0&1}\right]\quad\quad \left[\matrix{-1&0\cr0&-1}\right]$$ The final thing we can do with this definition of a $2\times2$ warping matrix is shear. If we want the output to be sheared along the first axis with $A$ and along the second with $B$, then we can use the matrix: $$\left[\matrix{1&A\cr B&1}\right]$$ To have one matrix representing any combination of these steps, you use matrix multiplication, see *note Merging multiple warpings::. So any combinations of these transformations can be displayed with one $2\times2$ matrix: $$\left[\matrix{a&b\cr c&d}\right]$$ The transformations above can cover a lot of the needs of most coordinate transformations. However they are limited to mapping the point $[\matrix{0&0}]$ to $[\matrix{0&0}]$. Therefore they are useless if you want one coordinate to be shifted compared to the other one. They are also space invariant, meaning that all the coordinates in the image will receive the same transformation. In other words, all the pixels in the output image will have the same area if placed over the input image. So transformations which require varying output pixel sizes like projections cannot be applied through this $2\times2$ matrix either (for example for the tilted ACS and WFC3 camera detectors on board the Hubble space telescope). To add these further capabilities, namely translation and projection, we use the homogeneous coordinates. They were defined about 200 years ago by August Ferdinand Möbius (1790 – 1868). For simplicity, we will only discuss points on a 2D plane and avoid the complexities of higher dimensions. We cannot provide a deep mathematical introduction here, interested readers can get a more detailed explanation from Wikipedia(2) and the references therein. By adding an extra coordinate to a point we can add the flexibility we need. The point $[\matrix{x&y}]$ can be represented as $[\matrix{xZ&yZ&Z}]$ in homogeneous coordinates. Therefore multiplying all the coordinates of a point in the homogeneous coordinates with a constant will give the same point. Put another way, the point $[\matrix{x&y&Z}]$ corresponds to the point $[\matrix{x/Z&y/Z}]$ on the constant $Z$ plane. Setting $Z=1$, we get the input image plane, so $[\matrix{u&v&1}]$ corresponds to $[\matrix{u&v}]$. With this definition, the transformations above can be generally written as: $$\left[\matrix{x\cr y\cr 1}\right]= \left[\matrix{a&b&0\cr c&d&0\cr 0&0&1}\right] \left[\matrix{u\cr v\cr 1}\right]$$ We thus acquired 4 extra degrees of freedom. By giving non-zero values to the zero valued elements of the last column we can have translation (try the matrix multiplication!). In general, any coordinate transformation that is represented by the matrix below is known as an affine transformation(3): $$\left[\matrix{a&b&c\cr d&e&f\cr 0&0&1}\right]$$ We can now consider translation, but the affine transform is still spatially invariant. Giving non-zero values to the other two elements in the matrix above gives us the projective transformation or Homography(4) which is the most general type of transformation with the $3\times3$ matrix: $$\left[\matrix{x'\cr y'\cr w}\right]= \left[\matrix{a&b&c\cr d&e&f\cr g&h&1}\right] \left[\matrix{u\cr v\cr 1}\right]$$ So the output coordinates can be calculated from: $$x={x' \over w}={au+bv+c \over gu+hv+1}\quad\quad\quad\quad y={y' \over w}={du+ev+f \over gu+hv+1}$$ Thus with Homography we can change the sizes of the output pixels on the input plane, giving a ‘perspective’-like visual impression. This can be quantitatively seen in the two equations above. When $g=h=0$, the denominator is independent of $u$ or $v$ and thus we have spatial invariance. Homography preserves lines at all orientations. A very useful fact about Homography is that its inverse is also a Homography. These two properties play a very important role in the implementation of this transformation. A short but instructive and illustrated review of affine, projective and also bi-linear mappings is provided in Heckbert 1989(5). ---------- Footnotes ---------- (1) These can be any real number, we are not necessarily talking about integer pixels here. (2) (3) (4) (5) Paul S. Heckbert. 1989. _Fundamentals of Texture mapping and Image Warping_, Master’s thesis at University of California, Berkeley. Note that since points are defined as row vectors there, the matrix is the transpose of the one discussed here.  File: gnuastro.info, Node: Merging multiple warpings, Next: Resampling, Prev: Warping basics, Up: Warp 6.4.2 Merging multiple warpings ------------------------------- In *note Warping basics:: we saw how a basic warp/transformation can be represented with a matrix. To make more complex warpings (for example to define a translation, rotation and scale as one warp) the individual matrices have to be multiplied through matrix multiplication. However matrix multiplication is not commutative, so the order of the set of matrices you use for the multiplication is going to be very important. The first warping should be placed as the left-most matrix. The second warping to the right of that and so on. The second transformation is going to occur on the warped coordinates of the first. As an example for merging a few transforms into one matrix, the multiplication below represents the rotation of an image about a point $[\matrix{U&V}]$ anticlockwise from the horizontal axis by an angle of $\theta$. To do this, first we take the origin to $[\matrix{U&V}]$ through translation. Then we rotate the image, then we translate it back to where it was initially. These three operations can be merged in one operation by calculating the matrix multiplication below: $$\left[\matrix{1&0&U\cr0&1&V\cr{}0&0&1}\right] \left[\matrix{cos\theta&-sin\theta&0\cr sin\theta&cos\theta&0\cr 0&0&1}\right] \left[\matrix{1&0&-U\cr0&1&-V\cr{}0&0&1}\right]$$  File: gnuastro.info, Node: Resampling, Next: Invoking astwarp, Prev: Merging multiple warpings, Up: Warp 6.4.3 Resampling ---------------- A digital image is composed of discrete ‘picture elements’ or ‘pixels’. When a real image is created from a camera or detector, each pixel’s area is used to store the number of photo-electrons that were created when incident photons collided with that pixel’s surface area. This process is called the ‘sampling’ of a continuous or analog data into digital data. When we change the pixel grid of an image or warp it as we defined in *note Warping basics::, we have to ‘guess’ the flux value of each pixel on the new grid based on the old grid, or re-sample it. Because of the ‘guessing’, any form of warping on the data is going to degrade the image and mix the original pixel values with each other. So if an analysis can be done on an un-warped data image, it is best to leave the image untouched and pursue the analysis. However as discussed in *note Warp:: this is not possible most of the times, so we have to accept the problem and re-sample the image. In most applications of image processing, it is sufficient to consider each pixel to be a point and not an area. This assumption can significantly speed up the processing of an image and also the simplicity of the code. It is a fine assumption when the signal to noise ratio of the objects are very large. The question will then be one of interpolation because you have multiple points distributed over the output image and you want to find the values at the pixel centers. To increase the accuracy, you might also sample more than one point from within a pixel giving you more points for a more accurate interpolation in the output grid. However, interpolation has several problems. The first one is that it will depend on the type of function you want to assume for the interpolation. For example you can choose a bi-linear or bi-cubic (the ‘bi’s are for the 2 dimensional nature of the data) interpolation method. For the latter there are various ways to set the constants(1). Such functional interpolation functions can fail seriously on the edges of an image. They will also need normalization so that the flux of the objects before and after the warpings are comparable. The most basic problem with such techniques is that they are based on a point while a detector pixel is an area. They add a level of subjectivity to the data (make more assumptions through the functions than the data can handle). For most applications this is fine, but in scientific applications where detection of the faintest possible galaxies or fainter parts of bright galaxies is our aim, we cannot afford this loss. Because of these reasons Warp will not use such interpolation techniques. Warp will do interpolation based on “pixel mixingâ€(2) or “area resamplingâ€. This is also what the Hubble Space Telescope pipeline calls “Drizzlingâ€(3). This technique requires no functions, it is thus non-parametric. It is also the closest we can get (make least assumptions) to what actually happens on the detector pixels. The basic idea is that you reverse-transform each output pixel to find which pixels of the input image it covers and what fraction of the area of the input pixels are covered. To find the output pixel value, you simply sum the value of each input pixel weighted by the overlap fraction (between 0 to 1) of the output pixel and that input pixel. Through this process, pixels are treated as an area not as a point (which is how detectors create the image), also the brightness (see *note Flux Brightness and magnitude::) of an object will be left completely unchanged. If there are very high spatial-frequency signals in the image (for example fringes) which vary on a scale smaller than your output image pixel size, pixel mixing can cause ailiasing(4). So if the input image has fringes, they have to be calculated and removed separately (which would naturally be done in any astronomical application). Because of the PSF no astronomical target has a sharp change in the signal so this issue is less important for astronomical applications, see *note PSF::. ---------- Footnotes ---------- (1) see for a nice introduction. (2) For a graphic demonstration see . (3) (4)  File: gnuastro.info, Node: Invoking astwarp, Prev: Resampling, Up: Warp 6.4.4 Invoking Warp ------------------- Warp an input dataset into a new grid. Any homographic warp (for example scaling, rotation, translation, projection) is acceptable, see *note Warping basics:: for the definitions. The general template for invoking Warp is: $ astwarp [OPTIONS...] InputImage One line examples: ## Rotate and then scale input image: $ astwarp --rotate=37.92 --scale=0.8 image.fits ## Scale, then translate the input image: $ astwarp --scale 8/3 --translate 2.1 image.fits ## Align raw image with celestial coordinates: $ astwarp --align rawimage.fits --output=aligned.fits ## Directly input a custom warping matrix (using fraction): $ astwarp --matrix=1/5,0,4/10,0,1/5,4/10,0,0,1 image.fits ## Directly input a custom warping matrix, with final numbers: $ astwarp --matrix="0.7071,-0.7071, 0.7071,0.7071" image.fits If any processing is to be done, Warp can accept one file as input. As in all Gnuastro programs, when an output is not explicitly set with the ‘--output’ option, the output filename will be set automatically based on the operation, see *note Automatic output::. For the full list of general options to all Gnuastro programs (including Warp), please see *note Common options::. To be the most accurate, the input image will be read as a 64-bit double precision floating point dataset and all internal processing is done in this format (including the raw output type). You can use the common ‘--type’ option to write the output in any type you want, see *note Numeric data types::. Warps must be specified as command-line options, either as (possibly multiple) modular warpings (for example ‘--rotate’, or ‘--scale’), or directly as a single raw matrix (with ‘--matrix’). If specified together, the latter (direct matrix) will take precedence and all the modular warpings will be ignored. Any number of modular warpings can be specified on the command-line and configuration files. If more than one modular warping is given, all will be merged to create one warping matrix. As described in *note Merging multiple warpings::, matrix multiplication is not commutative, so the order of specifying the modular warpings on the command-line, and/or configuration files makes a difference (see *note Configuration file precedence::). The full list of modular warpings and the other options particular to Warp are described below. The values to the warping options (modular warpings as well as ‘--matrix’), are a sequence of at least one number. Each number in this sequence is separated from the next by a comma (<,>). Each number can also be written as a single fraction (with a forward-slash between the numerator and denominator). Space and Tab characters are permitted between any two numbers, just don’t forget to quote the whole value. Otherwise, the value will not be fully passed onto the option. See the examples above as a demonstration. Based on the FITS standard, integer values are assigned to the center of a pixel and the coordinate [1.0, 1.0] is the center of the first pixel (bottom left of the image when viewed in SAO ds9). So the coordinate center [0.0, 0.0] is half a pixel away (in each axis) from the bottom left vertex of the first pixel. The resampling that is done in Warp (see *note Resampling::) is done on the coordinate axes and thus directly depends on the coordinate center. In some situations this if fine, for example when rotating/aligning a real image, all the edge pixels will be similarly affected. But in other situations (for example when scaling an over-sampled mock image to its intended resolution, this is not desired: you want the center of the coordinates to be on the corner of the pixel. In such cases, you can use the ‘--centeroncorner’ option which will shift the center by $0.5$ before the main warp, then shift it back by $-0.5$ after the main warp, see below. ‘-a’ ‘--align’ Align the image and celestial (WCS) axes given in the input. After it, the vertical image direction (when viewed in SAO ds9) corresponds to the declination and the horizontal axis is the inverse of the Right Ascension (RA). The inverse of the RA is chosen so the image can correspond to what you would actually see on the sky and is common in most survey images. Align is internally treated just like a rotation (‘--rotation’), but uses the input image’s WCS to find the rotation angle. Thus, if you have rotated the image before calling ‘--align’, you might get unexpected results (because the rotation is defined on the original WCS). ‘-r FLT’ ‘--rotate=FLT’ Rotate the input image by the given angle in degrees: $\theta$ in *note Warping basics::. Note that commonly, the WCS structure of the image is set such that the RA is the inverse of the image horizontal axis which increases towards the right in the FITS standard and as viewed by SAO ds9. So the default center for rotation is on the right of the image. If you want to rotate about other points, you have to translate the warping center first (with ‘--translate’) then apply your rotation and then return the center back to the original position (with another call to ‘--translate’, see *note Merging multiple warpings::. ‘-s FLT[,FLT]’ ‘--scale=FLT[,FLT]’ Scale the input image by the given factor(s): $M$ and $N$ in *note Warping basics::. If only one value is given, then both image axes will be scaled with the given value. When two values are given (separated by a comma), the first will be used to scale the first axis and the second will be used for the second axis. If you only need to scale one axis, use ‘1’ for the axis you don’t need to scale. The value(s) can also be written (on the command-line or in configuration files) as a fraction. ‘-f FLT[,FLT]’ ‘--flip=FLT[,FLT]’ Flip the input image around the given axis(s). If only one value is given, then both image axes are flipped. When two values are given (separated by a comma), you can choose which axis to flip over. ‘--flip’ only takes values ‘0’ (for no flip), or ‘1’ (for a flip). Hence, if you want to flip by the second axis only, use ‘--flip=0,1’. ‘-e FLT[,FLT]’ ‘--shear=FLT[,FLT]’ Shear the input image by the given value(s): $A$ and $B$ in *note Warping basics::. If only one value is given, then both image axes will be sheared with the given value. When two values are given (separated by a comma), the first will be used to shear the first axis and the second will be used for the second axis. If you only need to shear along one axis, use ‘0’ for the axis that must be untouched. The value(s) can also be written (on the command-line or in configuration files) as a fraction. ‘-t FLT[,FLT]’ ‘--translate=FLT[,FLT]’ Translate (move the center of coordinates) the input image by the given value(s): $c$ and $f$ in *note Warping basics::. If only one value is given, then both image axes will be translated by the given value. When two values are given (separated by a comma), the first will be used to translate the first axis and the second will be used for the second axis. If you only need to translate along one axis, use ‘0’ for the axis that must be untouched. The value(s) can also be written (on the command-line or in configuration files) as a fraction. ‘-p FLT[,FLT]’ ‘--project=FLT[,FLT]’ Apply a projection to the input image by the given values(s): $g$ and $h$ in *note Warping basics::. If only one value is given, then projection will apply to both axes with the given value. When two values are given (separated by a comma), the first will be used to project the first axis and the second will be used for the second axis. If you only need to project along one axis, use ‘0’ for the axis that must be untouched. The value(s) can also be written (on the command-line or in configuration files) as a fraction. ‘-m STR’ ‘--matrix=STR’ The warp/transformation matrix. All the elements in this matrix must be separated by comas(<,>) characters and as described above, you can also use fractions (a forward-slash between two numbers). The transformation matrix can be either a 2 by 2 (4 numbers), or a 3 by 3 (9 numbers) array. In the former case (if a 2 by 2 matrix is given), then it is put into a 3 by 3 matrix (see *note Warping basics::). The determinant of the matrix has to be non-zero and it must not contain any non-number values (for example infinities or NaNs). The elements of the matrix have to be written row by row. So for the general Homography matrix of *note Warping basics::, it should be called with ‘--matrix=a,b,c,d,e,f,g,h,1’. The raw matrix takes precedence over all the modular warping options listed above, so if it is called with any number of modular warps, the latter are ignored. ‘-c’ ‘--centeroncorer’ Put the center of coordinates on the corner of the first (bottom-left when viewed in SAO ds9) pixel. This option is applied after the final warping matrix has been finalized: either through modular warpings or the raw matrix. See the explanation above for coordinates in the FITS standard to better understand this option and when it should be used. ‘--hstartwcs=INT’ Specify the first header keyword number (line) that should be used to read the WCS information, see the full explanation in *note Invoking astcrop::. ‘--hendwcs=INT’ Specify the last header keyword number (line) that should be used to read the WCS information, see the full explanation in *note Invoking astcrop::. ‘-k’ ‘--keepwcs’ Do not correct the WCS information of the input image and save it untouched to the output image. By default the WCS (World Coordinate System) information of the input image is going to be corrected in the output image so the objects in the image are at the same WCS coordinates. But in some cases it might be useful to keep it unchanged (for example to correct alignments). ‘-C FLT’ ‘--coveredfrac=FLT’ Depending on the warp, the output pixels that cover pixels on the edge of the input image, or blank pixels in the input image, are not going to be fully covered by input data. With this option, you can specify the acceptable covered fraction of such pixels (any value between 0 and 1). If you only want output pixels that are fully covered by the input image area (and are not blank), then you can set ‘--coveredfrac=1’. Alternatively, a value of ‘0’ will keep output pixels that are even infinitesimally covered by the input(so the sum of the pixels in the input and output images will be the same).  File: gnuastro.info, Node: Data analysis, Next: Modeling and fittings, Prev: Data manipulation, Up: Top 7 Data analysis *************** Astronomical datasets (images or tables) contain very valuable information, the tools in this section can help in analyzing, extracting, and quantifying that information. For example getting general or specific statistics of the dataset (with *note Statistics::), detecting signal within a noisy dataset (with *note NoiseChisel::), or creating a catalog from an input dataset (with *note MakeCatalog::). * Menu: * Statistics:: Calculate dataset statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. * Match:: Match two datasets.  File: gnuastro.info, Node: Statistics, Next: NoiseChisel, Prev: Data analysis, Up: Data analysis 7.1 Statistics ============== The distribution of values in a dataset can provide valuable information about it. For example, in an image, if it is a positively skewed distribution, we can see that there is significant data in the image. If the distribution is roughly symmetric, we can tell that there is no significant data in the image. In a table, when we need to select a sample of objects, it is important to first get a general view of the whole sample. On the other hand, you might need to know certain statistical parameters of the dataset. For example, if we have run a detection algorithm on an image, and we want to see how accurate it was, one method is to calculate the average of the undetected pixels and see how reasonable it is (if detection is done correctly, the average of undetected pixels should be approximately equal to the background value, see *note Sky value::). In a table, you might have calculated the magnitudes of a certain class of objects and want to get some general characteristics of the distribution immediately on the command-line (very fast!), to possibly change some parameters. The Statistics program is designed for such situations. * Menu: * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of $\sigma$-clipping. * Sky value:: Definition and derivation of the Sky value. * Invoking aststatistics:: Arguments and options to Statistics.  File: gnuastro.info, Node: Histogram and Cumulative Frequency Plot, Next: Sigma clipping, Prev: Statistics, Up: Statistics 7.1.1 Histogram and Cumulative Frequency Plot --------------------------------------------- Histograms and the cumulative frequency plots are both used to visually study the distribution of a dataset. A histogram shows the number of data points which lie within pre-defined intervals (bins). So on the horizontal axis we have the bin centers and on the vertical, the number of points that are in that bin. You can use it to get a general view of the distribution: which values have been repeated the most? how close/far are the most significant bins? Are there more values in the larger part of the range of the dataset, or in the lower part? Similarly, many very important properties about the dataset can be deduced from a visual inspection of the histogram. In the Statistics program, the histogram can be either output to a table to plot with your favorite plotting program(1), or it can be shown with ASCII characters on the command-line, which is very crude, but good enough for a fast and on-the-go analysis, see the example in *note Invoking aststatistics::. The width of the bins is only necessary parameter for a histogram. In the limiting case that the bin-widths tend to zero (while assuming the number of points in the dataset tend to infinity), then the histogram will tend to the probability density function (https://en.wikipedia.org/wiki/Probability_density_function) of the distribution. When the absolute number of points in each bin is not relevant to the study (only the shape of the histogram is important), you can _normalize_ a histogram so like the probability density function, the sum of all its bins will be one. In the cumulative frequency plot of a distribution, the horizontal axis is the sorted data values and the y axis is the index of each data in the sorted distribution. Unlike a histogram, a cumulative frequency plot does not involve intervals or bins. This makes it less prone to any sort of bias or error that a given bin-width would have on the analysis. When a larger number of the data points have roughly the same value, then the cumulative frequency plot will become steep in that vicinity. This occurs because on the horizontal axis, there is little change while on the vertical axis, the indexes constantly increase. Normalizing a cumulative frequency plot means to divide each index (y axis) by the total number of data points (or the last value). Unlike the histogram which has a limited number of bins, ideally the cumulative frequency plot should have one point for every data element. Even in small datasets (for example a $200\times200$ image) this will result in an unreasonably large number of points to plot (40000)! As a result, for practical reasons, it is common to only store its value on a certain number of points (intervals) in the input range rather than the whole dataset, so you should determine the number of bins you want when asking for a cumulative frequency plot. In Gnuastro (and thus the Statistics program), the number reported for each bin is the total number of data points until the larger interval value for that bin. You can see an example histogram and cumulative frequency plot of a single dataset under the ‘--asciihist’ and ‘--asciicfp’ options of *note Invoking aststatistics::. So as a summary, both the histogram and cumulative frequency plot in Statistics will work with bins. Within each bin/interval, the lower value is considered to be within then bin (it is inclusive), but its larger value is not (it is exclusive). Formally, an interval/bin between a and b is represented by [a, b). When the over-all range of the dataset is specified (with the ‘--greaterequal’, ‘--lessthan’, or ‘--qrange’ options), the acceptable values of the dataset are also defined with a similar inclusive-exclusive manner. But when the range is determined from the actual dataset (none of these options is called), the last element in the dataset is included in the last bin’s count. ---------- Footnotes ---------- (1) We recommend PGFPlots (http://pgfplots.sourceforge.net/) which generates your plots directly within TeX (the same tool that generates your document).  File: gnuastro.info, Node: Sigma clipping, Next: Sky value, Prev: Histogram and Cumulative Frequency Plot, Up: Statistics 7.1.2 Sigma clipping -------------------- Let’s assume that you have pure noise (centered on zero) with a clear Gaussian distribution (https://en.wikipedia.org/wiki/Normal_distribution), or see *note Photon counting noise::. Now let’s assume you add very bright objects (signal) on the image which have a very sharp boundary. By a sharp boundary, we mean that there is a clear cutoff (from the noise) at the pixels the objects finish. In other words, at their boundaries, the objects do not fade away into the noise. In such a case, when you plot the histogram (see *note Histogram and Cumulative Frequency Plot::) of the distribution, the pixels relating to those objects will be clearly separate from pixels that belong to parts of the image that did not have any signal (were just noise). In the cumulative frequency plot, after a steady rise (due to the noise), you would observe a long flat region were for a certain range of data (horizontal axis), there is no increase in the index (vertical axis). Outliers like the example above can significantly bias the measurement of noise statistics. $\sigma$-clipping is defined as a way to avoid the effect of such outliers. In astronomical applications, cosmic rays (when they collide at a near normal incidence angle) are a very good example of such outliers. The tracks they leave behind in the image are perfectly immune to the blurring caused by the atmosphere and the aperture. They are also very energetic and so their borders are usually clearly separated from the surrounding noise. So $\sigma$-clipping is very useful in removing their effect on the data. See Figure 15 in Akhlaghi and Ichikawa, 2015 (https://arxiv.org/abs/1505.01664). $\sigma$-clipping is defined as the very simple iteration below. In each iteration, the range of input data might decrease and so when the outliers have the conditions above, the outliers will be removed through this iteration. The exit criteria will be discussed below. 1. Calculate the standard deviation ($\sigma$) and median ($m$) of a distribution. 2. Remove all points that are smaller or larger than $m\pm\alpha\sigma$. 3. Go back to step 1, unless the selected exit criteria is reached. The reason the median is used as a reference and not the mean is that the mean is too significantly affected by the presence of outliers, while the median is less affected, see *note Quantifying signal in a tile::. As you can tell from this algorithm, besides the condition above (that the signal have clear high signal to noise boundaries) $\sigma$-clipping is only useful when the signal does not cover more than half of the full data set. If they do, then the median will lie over the outliers and $\sigma$-clipping might remove the pixels with no signal. There are commonly two exit criteria to stop the $\sigma$-clipping iteration: • When a certain number of iterations has taken place (second value to the ‘--sigclip’ option is larger than 1). • When the new measured standard deviation is within a certain tolerance level of the old one (second value to the ‘--sigclip’ option is less than 1). The tolerance level is defined by: $$\sigma_{old}-\sigma_{new} \over \sigma_{new}$$ The standard deviation is used because it is heavily influenced by the presence of outliers. Therefore the fact that it stops changing between two iterations is a sign that we have successfully removed outliers. Note that in each clipping, the dispersion in the distribution is either less or equal. So $\sigma_{old}\geq\sigma_{new}$. When working on astronomical images, objects like galaxies and stars are blurred by the atmosphere and the telescope aperture, therefore their signal sinks into the noise very gradually. Galaxies in particular do not appear to have a clear high signal to noise cutoff at all. Therefore $\sigma$-clipping will not be useful in removing their effect on the data. To gauge if $\sigma$-clipping will be useful for your dataset, look at the histogram (see *note Histogram and Cumulative Frequency Plot::). The ASCII histogram that is printed on the command-line with ‘--asciihist’ is good enough in most cases.  File: gnuastro.info, Node: Sky value, Next: Invoking aststatistics, Prev: Sigma clipping, Up: Statistics 7.1.3 Sky value --------------- One of the most important aspects of a dataset is its reference value: the value of the dataset where there is no signal. Without knowing, and thus removing the effect of, this value it is impossible to compare the derived results of many high-level analyses over the dataset with other datasets (in the attempt to associate our results with the “real†world). In astronomy, this reference value is known as the “Sky†value: the value where there is no signal from objects (for example galaxies, stars, planets or comets). Depending on the dataset, the Sky value maybe a fixed value over the whole dataset, or it may vary based on location. For an example of the latter case, see Figure 11 in Akhlaghi and Ichikawa (2015) (https://arxiv.org/abs/1505.01664). Because of the significance of the Sky value in astronomical data analysis, we have devoted this subsection to it for a thorough review. We start with a thorough discussion on its definition (*note Sky value definition::). In the astronomical literature, researchers use a variety of methods to estimate the Sky value, so in *note Sky value misconceptions::) we review those and discuss their biases. From the definition of the Sky value, the most accurate way to estimate the Sky value is to run a detection algorithm (for example *note NoiseChisel::) over the dataset and use the un-detected pixels. However, there is also a more crude method that maybe useful when good direct detection is not initially possible (for example due to too many cosmic rays in a shallow image). A more crude (but simpler method) that is usable in such situations is discussed in *note Quantifying signal in a tile::. * Menu: * Sky value definition:: Definition of the Sky/reference value. * Sky value misconceptions:: Wrong methods to estimate the Sky value. * Quantifying signal in a tile:: Method to estimate the presence of signal.  File: gnuastro.info, Node: Sky value definition, Next: Sky value misconceptions, Prev: Sky value, Up: Sky value 7.1.3.1 Sky value definition ............................ This analysis is taken from Akhlaghi and Ichikawa (2015) (https://arxiv.org/abs/1505.01664). Let’s assume that all instrument defects – bias, dark and flat – have been corrected and the brightness (see *note Flux Brightness and magnitude::) of a detected object, $O$, is desired. The sources of flux on pixel $i$(1) of the image can be written as follows: • Contribution from the target object, ($O_i$). • Contribution from other detected objects, ($D_i$). • Undetected objects or the fainter undetected regions of bright objects, ($U_i$). • A cosmic ray, ($C_i$). • The background flux, which is defined to be the count if none of the others exists on that pixel, ($B_i$). The total flux in this pixel ($T_i$) can thus be written as: $$T_i=B_i+D_i+U_i+C_i+O_i.$$ By definition, $D_i$ is detected and it can be assumed that it is correctly estimated (deblended) and subtracted, thus $D_i=0$. There are also methods to detect and remove cosmic rays, for example the method described in van Dokkum (2001)(2), or by comparing multiple exposures. This allows us to set $C_i=0$. Note that in practice, $D_i$ and $U_i$ are correlated, because they both directly depend on the detection algorithm and its input parameters. Also note that no detection or cosmic ray removal algorithm is perfect. With these limitations in mind, the observed Sky value for this pixel ($S_i$) can be defined as $$S_i=B_i+U_i.$$ Therefore, as the detection process (algorithm and input parameters) becomes more accurate, or $U_i\to0$, the sky value will tend to the background value or $S_i\to B_i$. Therefore, while $B_i$ is an inherent property of the data (pixel in an image), $S_i$ depends on the detection process. Over a group of pixels, for example in an image or part of an image, this equation translates to the average of undetected pixels. With this definition of sky, the object flux in the data can be calculated with $$T_{i}=S_{i}+O_{i} \quad\rightarrow\quad O_{i}=T_{i}-S_{i}.$$ Hence, the more accurately $S_i$ is measured, the more accurately the brightness (sum of pixel values) of the target object can be measured (photometry). Any under-(over-)estimation in the sky will directly translate to an over-(under-)estimation of the measured object’s brightness. In the fainter outskirts of an object a very small fraction of the photo-electrons in the pixels actually belong to objects (see Figure 1b in Akhlaghi and Ichikawa (2015) (https://arxiv.org/abs/1505.01664)). Therefore even a small over estimation of the sky value will result in the loss of a very large portion of most galaxies. Besides the lost area/brightness, this will also cause an over-estimation of the Sky value and thus even more under-estimation of the object’s brightness. It is thus very important to detect the diffuse flux of a target, even if they are not your primary target. The *Sky value* is only correctly found when all the detected objects ($D_i$ and $C_i$) have been removed from the data. ---------- Footnotes ---------- (1) For this analysis the dimension of the data (image) is irrelevant. So if the data is an image (2D) with width of $w$ pixels, then a pixel located on column $x$ and row $y$ (where all counting starts from zero and (0, 0) is located on the bottom left corner of the image), would have an index: $i=x+y\times{}w$. (2) van Dokkum, P. G. (2001). Publications of the Astronomical Society of the Pacific. 113, 1420.  File: gnuastro.info, Node: Sky value misconceptions, Next: Quantifying signal in a tile, Prev: Sky value definition, Up: Sky value 7.1.3.2 Sky value misconceptions ................................ As defined in *note Sky value::, the sky value is only accurately defined when the detection algorithm is not significantly reliant on the sky value. In particular its detection threshold. However, most signal-based detection tools(1) use the sky value as a reference to define the detection threshold. So these old techniques had to rely on approximations based on other assumptions about the data. A review of those other techniques can be seen in Appendix A of Akhlaghi and Ichikawa (2015)(2). Since they were extensively used in astronomical data analysis for several decades, such approximations have given rise to a lot of misconceptions, ambiguities and disagreements about the sky value and how to measure it. As a summary, the major methods used until now were an approximation of the mode of the image pixel distribution and $\sigma$-clipping. • To find the mode of a distribution those methods would either have to assume (or find) a certain probability density function (PDF) or use the histogram. But astronomical datasets can have any distribution, making it almost impossible to define a generic function. Also, histogram-based results are very inaccurate (there is a large dispersion) and it depends on the histogram bin-widths. • Another approach was to iteratively clip the brightest pixels in the image (which is known as $\sigma$-clipping, since the reference was found from the image mean and its standard deviation or $\sigma$). See *note Sigma clipping:: for a complete explanation. The problem with $\sigma$-clipping was that real astronomical objects have diffuse and faint wings that penetrate deeply into the noise. So only removing their brightest parts is completely useless in removing the systematic bias an object’s fainter parts cause in the sky value. As discussed in *note Sky value::, the sky value can only be correctly defined as the average of undetected pixels. Therefore all such approaches that try to approximate the sky value prior to detection are ultimately poor approximations. ---------- Footnotes ---------- (1) According to Akhlaghi and Ichikawa (2015), signal-based detection is a detection process that relies heavily on assumptions about the to-be-detected objects. This method was the most heavily used technique prior to the introduction of NoiseChisel in that paper. (2) Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.  File: gnuastro.info, Node: Quantifying signal in a tile, Prev: Sky value misconceptions, Up: Sky value 7.1.3.3 Quantifying signal in a tile .................................... Put simply, noise can characterized with a certain spread about a characteristic value. In the Gaussian distribution (most commonly used to model noise) the spread is defined by the standard deviation about the characteristic mean. Before continuing let’s clarify some definitions first: _Data_ is defined as the combination of signal and noise (so a noisy image is one _data_-set). _Signal_ is defined as the mean of the noise on each element (after sky subtraction, see *note Sky value definition::). Let’s assume that the _background_ (see *note Sky value definition::) is subtracted and is zero. When a data set doesn’t have any signal (only noise), the mean, median and mode of the distribution are equal within statistical errors and approximately equal to the background value. Signal always has a positive value and will never become negative, see Figure 1 in Akhlaghi and Ichikawa (2015) (https://arxiv.org/abs/1505.01664). Therefore, as more signal is added to the raw noise, the mean, median and mode of the dataset (which has both signal and noise) shift to the positive. The mean’s shift is the largest. The median shifts less, since it is defined based on an ordered distribution and so is not affected by a small number of outliers. The distribution’s mode shifts the least to the positive. Inverting the argument above gives us a robust method to quantify the significance of signal in a dataset. Namely, when the mode and median of a distribution are approximately equal, we can argue that there is no significant signal. To allow for gradients (which are commonly present in ground-based images), we can consider the image to be made of a grid of tiles (see *note Tessellation::(1)). Hence, from the difference of the mode and median on each tile, we can ‘detect’ the significance of signal in it. The median of a distribution is defined to be the value of the distribution’s middle point after sorting (or 0.5 quantile). Thus, to estimate the presence of signal, we’ll compare with the quantile of the mode with 0.5, if the difference is larger than the value given to the ‘--modmedqdiff’ option, this tile will be ignored. You can read this option as “mode-median-quantile-diffâ€. This method to use the input’s skewness is possible because of a new algorithm to find the mode of a distribution that was defined in Appendix C of Akhlaghi and Ichikawa (2015). However, the raw dataset’s distribution is noisy (noise also affects the sorting), so using the argument above on the raw input will give a noisy result. To decrease the noise/error in estimating the mode, we will use convolution (see *note Convolution process::). Convolution decreases the range of the dataset and enhances its skewness, See Section 3.1.1 and Figure 4 in Akhlaghi and Ichikawa (2015). This enhanced skewness can be interpreted as an increase in the Signal to noise ratio of the objects buried in the noise. Therefore, to obtain an even better measure of the presence of signal in a mesh, the image can be convolved with a given kernel first. Note that through the difference of the mode and median we have actually ‘detected’ data in the distribution. However this “detection†was only based on the total distribution of the data in each tile (a much lower resolution). This is the main limitation of this technique. The best approach is thus to do detection over the dataset, mask all the detected pixels and use the undetected regions to estimate the sky and its standard deviation. The mean value of the tiles that have an approximately equal mode and median will be the Sky value. However there is one final hurdle: astronomical datasets are commonly plagued with Cosmic rays. Images of Cosmic rays aren’t smoothed by the atmosphere or telescope aperture, so they have sharp boundaries. Also, since they don’t occupy too many pixels, they don’t affect the mode and median calculation. But their very high values can greatly bias the calculation of the mean (recall how the mean shifts the fastest in the presence of outliers), see Figure 15 in Akhlaghi and Ichikawa (2015) for one example. The effect of outliers like cosmic rays on the mean and standard deviation can be removed through $\sigma$-clipping, see *note Sigma clipping:: for a complete explanation. Therefore, after asserting that the mode and median are approximately equal in a tile (see *note Tessellation::), the final Sky value and its standard deviation are determined after $\sigma$-clipping with the ‘--sigmaclip’ option. ---------- Footnotes ---------- (1) The options to customize the tessellation are discussed in *note Processing options::.  File: gnuastro.info, Node: Invoking aststatistics, Prev: Sky value, Up: Statistics 7.1.4 Invoking Statistics ------------------------- Statistics will print statistical measures of an input dataset (table column or image). The executable name is ‘aststatistics’ with the following general template $ aststatistics [OPTION ...] InputImage.fits One line examples: ## Print some general statistics of input image: $ aststatistics image.fits ## Print some general statistics of column named MAG_F160W: $ aststatistics catalog.fits -h1 --column=MAG_F160W ## Make the histogram of the column named MAG_F160W: $ aststatistics table.fits -cMAG_F160W --histogram ## Find the Sky value on image with a given kernel: $ aststatistics image.fits --sky --kernel=kernel.fits ## Print Sigma-clipped results of records with a MAG_F160W ## column value between 26 and 27: $ aststatistics cat.fits -cMAG_F160W -g26 -l27 --sigmaclip=3,0.2 ## Print the median value of all records in column MAG_F160W that ## have a value larger than 3 in column PHOTO_Z: $ aststatistics tab.txt -rPHOTO_Z -g3 -cMAG_F160W --median An input image or table is necessary when processing is to be done. If any output file is to be created, the value to the ‘--output’ option, is used as the base name for the generated files. Without ‘--output’, the input name will be used to generate an output name, see *note Automatic output::. The options described below are particular to Statistics, but for general operations, it shares a large collection of options with the other Gnuastro programs, see *note Common options:: for the full list. Options can also be given in configuration files, for more, please see *note Configuration files::. The input dataset may have blank values (see *note Blank pixels::), in this case, all blank pixels are ignored during the calculation. Initially, the full dataset will be read, but it is possible to select a specific range of data elements to use in the analysis of each run. You can either directly specify a minimum and maximum value for the range of data elements to use (with ‘--greaterequal’ or ‘--lessthan’), or specify the range using quantiles (with ‘--qrange’). If a range is specified, all pixels outside of it are ignored before any processing. The following set of options are for specifying the input/outputs of Statistics. There are many other input/output options that are common to all Gnuastro programs including Statistics, see *note Input output options:: for those. ‘-c STR/INT’ ‘--column=STR/INT’ The input column selector when the input file is a table. See *note Selecting table columns:: for a full description of how to use this option. For more on how tables are read in Gnuastro, please see *note Tables::. ‘-r STR/INT’ ‘--refcol=STR/INT’ The reference column selector when the input file is a table. When a reference column is given, the range options below will be applied to this column and only elements in the input column that have a reference value in the correct range will be used. In practice this option allows you to select a subset of the input column based on values in another (the reference) column. All the statistical calculations will be done on the selected input column, not the reference column. ‘-g FLT’ ‘--greaterequal=FLT’ Limit the range of inputs into those with values greater and equal to what is given to this option. None of the values below this value will be used in any of the processing steps below. ‘-l FLT’ ‘--lessthan=FLT’ Limit the range of inputs into those with values less-than what is given to this option. None of the values greater or equal to this value will be used in any of the processing steps below. ‘-Q FLT[,FLT]’ ‘--qrange=FLT[,FLT]’ Specify the range of usable inputs using the quantile. This option can take one or two quantiles to specify the range. When only one number is input (let’s call it $Q$), the range will be those values in the quantile range $Q$ to $1-Q$. So when only one value is given, it must be less than 0.5. When two values are given, the first is used as the lower quantile range and the second is used as the larger quantile range. The quantile of a given element in a dataset is defined by the fraction of its index to the total number of values in the sorted input array. So the smallest and largest values in the dataset have a quantile of 0.0 and 1.0. The quantile is a very useful non-parametric (making no assumptions about the input) relative measure to specify a range. It can best be understood in terms of the cumulative frequency plot, see *note Histogram and Cumulative Frequency Plot::. The quantile of each horizontal axis value in the cumulative frequency plot is the vertical axis value associate with it. When no operation is requested, Statistics will print some general basic properties of the input dataset on the command-line like the example below (ran on one of the output images of ‘make check’(1)). This default behavior is designed to help give you a general feeling of how the data are distributed and help in narrowing down your analysis. $ aststatistics convolve_spatial_scaled_noised.fits \ --greaterequal=9500 --lessthan=11000 Statistics (GNU Astronomy Utilities) X.X ------- Input: convolve_spatial_scaled_noised.fits (hdu: 0) Range: from (inclusive) 9500, upto (exclusive) 11000. Unit: Brightness ------- Number of elements: 9074 Minimum: 9622.35 Maximum: 10999.7 Mode: 10055.45996 Mode quantile: 0.4001983908 Median: 10093.7 Mean: 10143.98257 Standard deviation: 221.80834 ------- Histogram: | ** | ****** | ******* | ********* | ************* | ************** | ****************** | ******************** | *************************** * | ***************************************** *** |* ************************************************************** |----------------------------------------------------------------- Gnuastro’s Statistics is a very general purpose program, so to be able to easily understand this diversity in its operations (and how to possibly run them together), we’ll divided the operations into two types: those that don’t respect the position of the elements and those that do (by tessellating the input on a tile grid, see *note Tessellation::). The former treat the whole dataset as one and can re-arrange all the elements (for example sort them), but the former do their processing on each tile independently. First, we’ll review the operations that work on the whole dataset. The group of options below can used to get a single value measurement of the whole dataset. They will print only the requested value as one field in a line/row, like the ‘--mean’, ‘--median’ options. These options can be called any number of times and in any order. The outputs of all such options will be printed on one line following each other (with a space character between them). This feature makes these options very useful in scripts, or to redirect into programs like GNU AWK for higher-level processing. These are some of the most basic measures, Gnuastro is still under heavy development and this list will grow. If you want another statistical parameter, please contact us and we will do out best to add it to this list, see *note Suggest new feature::. ‘-n’ ‘--number’ Print the number of all used (non-blank and in range) elements. ‘--minimum’ Print the minimum value of all used elements. ‘--maximum’ Print the maximum value of all used elements. ‘--sum’ Print the sum of all used elements. ‘-m’ ‘--mean’ Print the mean (average) of all used elements. ‘-t’ ‘--std’ Print the standard deviation of all used elements. ‘-E’ ‘--median’ Print the median of all used elements. ‘-u FLT[,FLT[,...]]’ ‘--quantile=FLT[,FLT[,...]]’ Print the values at the given quantiles of the input dataset. Any number of quantiles may be given and one number will be printed for each. Values can either be written as a single number or as fractions, but must be between zero and one (inclusive). Hence, in effect ‘--quantile=0.25 --quantile=0.75’ is equivalent to ‘--quantile=0.25,3/4’, or ‘-u1/4,3/4’. The returned value is one of the elements from the dataset. Taking $q$ to be your desired quantile, and $N$ to be the total number of used (non-blank and within the given range) elements, the returned value is at the following position in the sorted array: $round(q\times{}N$). ‘--quantfunc=FLT[,FLT[,...]]’ Print the quantiles of the given values in the dataset. This option is the inverse of the ‘--quantile’ and operates similarly except that the acceptable values are within the range of the dataset, not between 0 and 1. Formally it is known as the “Quantile functionâ€. Since the dataset is not continuous this function will find the nearest element of the dataset and use its position to estimate the quantile function. ‘-O’ ‘--mode’ Print the mode of all used elements. The mode is found through the mirror distribution which is fully described in Appendix C of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664). See that section for a full description. This mode calculation algorithm is non-parametric, so when the dataset is not large enough (larger than about 1000 elements usually), or doesn’t have a clear mode it can fail. In such cases, this option will return a value of ‘nan’ (for the floating point NaN value). As described in that paper, the easiest way to assess the quality of this mode calculation method is to use it’s symmetricity (see ‘--modesym’ below). A better way would be to use the ‘--mirror’ option to generate the histogram and cumulative frequency tables for any given mirror value (the mode in this case) as a table. If you generate plots like those shown in Figure 21 of that paper, then your mode is accurate. ‘--modequant’ Print the quantile of the mode. You can get the actual mode value from the ‘--mode’ described above. In many cases, the absolute value of the mode is irrelevant, but its position within the distribution is important. In such cases, this option will become handy. ‘--modesym’ Print the symmetricity of the calculated mode. See the description of ‘--mode’ for more. This mode algorithm finds the mode based on how symmetric it is, so if the symmetricity returned by this option is too low, the mode is not too accurate. See Appendix C of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664) for a full description. In practice, symmetricity values larger than 0.2 are mostly good. ‘--modesymvalue’ Print the value in the distribution where the mirror and input distributions are no longer symmetric, see ‘--mode’ and Appendix C of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664) for more. The list of options below are for those statistical operations that output more than one value. So while they can be called together in one run, their outputs will be distinct (each one’s output will usually be printed in more than one line). ‘-A’ ‘--asciihist’ Print an ASCII histogram of the usable values within the input dataset along with some basic information like the example below (from the UVUDF catalog(2)). The width and height of the histogram (in units of character widths and heights on your command-line terminal) can be set with the ‘--numasciibins’ (for the width) and ‘--asciiheight’ options. For a full description of the histogram, please see *note Histogram and Cumulative Frequency Plot::. An ASCII plot is certainly very crude and cannot be used in any publication, but it is very useful for getting a general feeling of the input dataset very fast and easily on the command-line without having to take your hands off the keyboard (which is a major distraction!). If you want to try it out, you can write it all in one line and ignore the <\> and extra spaces. $ aststatistics uvudf_rafelski_2015.fits.gz --hdu=1 \ --column=MAG_F160W --lessthan=40 \ --asciihist --numasciibins=55 ASCII Histogram: Number: 8593 Y: (linear: 0 to 660) X: (linear: 17.7735 -- 31.4679, in 55 bins) | **** | ***** | ****** | ******** | ********* | *********** | ************** | ***************** | *********************** | ******************************** |*** *************************************************** |------------------------------------------------------- ‘--asciicfp’ Print the cumulative frequency plot of the usable elements in the input dataset. Please see descriptions under ‘--asciihist’ for more, the example below is from the same input table as that example. To better understand the cumulative frequency plot, please see *note Histogram and Cumulative Frequency Plot::. $ aststatistics uvudf_rafelski_2015.fits.gz --hdu=1 \ --column=MAG_F160W --lessthan=40 \ --asciicfp --numasciibins=55 ASCII Cumulative frequency plot: Y: (linear: 0 to 8593) X: (linear: 17.7735 -- 31.4679, in 55 bins) | ******* | ********** | *********** | ************* | ************** | *************** | ***************** | ******************* | *********************** | ****************************** |******************************************************* |------------------------------------------------------- ‘-H’ ‘--histogram’ Save the histogram of the usable values in the input dataset into a table. The first column is the value at the center of the bin and the second is the number of points in that bin. If the ‘--cumulative’ option is also called with this option in a run, then the table will have three columns (the third is the cumulative frequency plot). Through the ‘--numbins’ and ‘--lowerbin’ you can modify the first column values and with ‘--normalize’ and ‘--maxbinone’ you can modify the second columns. See below for the description of each. By default (when no ‘--output’ is specified) a plain text table will be created, see *note Gnuastro text table format::. If a FITS name is specified, you can use the common option ‘--tableformat’ to have it as a FITS ASCII or FITS binary format, see *note Common options::. This table can then be fed into your favorite plotting tool and get a much more clean and nice histogram than what the raw command-line can offer you (with the ‘--asciihist’ option). ‘-C’ ‘--cumulative’ Save the cumulative frequency plot of the usable values in the input dataset into a table, similar to ‘--histogram’. ‘-s’ ‘--sigmaclip’ Do $\sigma$-clipping on the usable pixels of the input dataset. See *note Sigma clipping:: for a full description on $\sigma$-clipping and also to better understand this option. The $\sigma$-clipping parameters can be set through the ‘--sclipparams’ option (see below). ‘--mirror=FLT’ Make a histogram and cumulative frequency plot of the mirror distribution for the given dataset when the mirror is located at the value to this option. The mirror distribution is fully described in Appendix C of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664) and currently it is only used to calculate the mode (see ‘--mode’). Just note that the mirror distribution is a discrete distribution like the input, so while you may give any number as the value to this option, the actual mirror value is the closest number in the input dataset to this value. If the two numbers are different, Statistics will warn you of the actual mirror value used. This option will make a table as output. Depending on your selected name for the output, it will be either a FITS table or a plain text table (which is the default). It contains three columns: the first is the center of the bins, the second is the histogram (with the largest value set to 1) and the third is the normalized cumulative frequency plot of the mirror distribution. The bins will be positioned such that the mode is on the starting interval of one of the bins to make it symmetric around the mirror. With this output file and the input histogram (that you can generate in another run of Statistics, using the ‘--onebinvalue’), it is possible to make plots like Figure 21 of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664). The list of options below allow customization of the histogram and cumulative frequency plots (for the ‘--histogram’, ‘--cumulative’, ‘--asciihist’, and ‘--asciicfp’ options). ‘--numbins’ The number of bins (rows) to use in the histogram and the cumulative frequency plot tables (outputs of ‘--histogram’ and ‘--cumulative’). ‘--numasciibins’ The number of bins (characters) to use in the ASCII plots when printing the histogram and the cumulative frequency plot (outputs of ‘--asciihist’ and ‘--asciicfp’). ‘--asciiheight’ The number of lines to use when printing the ASCII histogram and cumulative frequency plot on the command-line (outputs of ‘--asciihist’ and ‘--asciicfp’). ‘-n’ ‘--normalize’ Normalize the histogram or cumulative frequency plot tables (outputs of ‘--histogram’ and ‘--cumulative’). For a histogram, the sum of all bins will become one and for a cumulative frequency plot the last bin value will be one. ‘--maxbinone’ Divide all the histogram values by the maximum bin value so it becomes one and the rest are similarly scaled. In some situations (for example if you want to plot the histogram and cumulative frequency plot in one plot) this can be very useful. ‘--onebinstart=FLT’ Make sure that one bin starts with the value to this option. In practice, this will shift the bins used to find the histogram and cumulative frequency plot such that one bin’s lower interval becomes this value. For example when the histogram range includes negative and positive values and zero has a special significance in your analysis, then zero will be somewhere in one bin and will mix counts of positive and negative. By setting ‘--onebinstart=0’, you can make sure that the viewers of the histogram will not be confused without doing the math of setting a range and number of bins. Note that by default, the first row of the histogram and cumulative frequency plot show the central values of each bin. So in the example above you will not see the 0.000 in the first column, you will see two symmetric values. If the value is not within the usable input range, this option will be ignored. All the options described until now were from the first class of operations discussed above: those that treat the whole dataset as one. However. It often happens that the relative position of the dataset elements over the dataset is significant. For example you don’t want one median value for the whole input image, you want to know how the median changes over the image. For such operations, the input has to be tessellated (see *note Tessellation::). Thus this class of options can’t currently be called along with the options above in one run of Statistics. ‘-t’ ‘--ontile’ Do the respective single-valued calculation over one tile of the input dataset, not the whole dataset. This option must be called with at least one of the single valued options discussed above (for example ‘--mean’ or ‘--quantile’). The output will be a file in the same format as the input. If the ‘--oneelempertile’ option is called, then one element/pixel will be used for each tile (see *note Processing options::). Otherwise, the output will have the same size as the input, but each element will have the value corresponding to that tile’s value. If multiple single valued operations are called, then for each operation there will be one extension in the output FITS file. ‘-y’ ‘--sky’ Estimate the Sky value on each tile as fully described in *note Quantifying signal in a tile::. As described in that section, several options are necessary to configure the Sky estimation which are listed below. The output file will have two extensions: the first is the Sky value and the second is the Sky standard deviation on each tile. Similar to ‘--ontile’, if the ‘--oneelempertile’ option is called, then one element/pixel will be used for each tile (see *note Processing options::). The parameters for estimating the sky value can be set with the following options, except for the ‘--sclipparams’ option (which is also used by the ‘--sigmaclip’), the rest are only used for the Sky value estimation. ‘-k=STR’ ‘--kernel=STR’ File name of kernel to help in estimating the significance of signal in a tile, see *note Quantifying signal in a tile::. ‘--khdu=STR’ Kernel HDU to help in estimating the significance of signal in a tile, see *note Quantifying signal in a tile::. ‘--mirrordist=FLT’ Maximum distance (as a multiple of error) to estimate the difference between the input and mirror distributions in finding the mode, see Appendix C of Akhlaghi and Ichikawa 2015 (https://arxiv.org/abs/1505.01664), also see *note Quantifying signal in a tile::. ‘--modmedqdiff=FLT’ The maximum acceptable distance between the mode and median, see *note Quantifying signal in a tile::. ‘--sclipparams=FLT,FLT’ The $\sigma$-clipping parameters, see *note Sigma clipping::. This option takes two values which are separated by a comma (<,>). Each value can either be written as a single number or as a fraction of two numbers (for example ‘3,1/10’). The first value to this option is the multiple of $\sigma$ that will be clipped ($\alpha$ in that section). The second value is the exit criteria. If it is less than 1, then it is interpreted as tolerance and if it is larger than one it is a specific number. Hence, in the latter case the value must be an integer. ‘--smoothwidth=INT’ Width of a flat kernel to convolve the interpolated tile values. Tile interpolation is done using the median of the ‘--interpnumngb’ neighbors of each tile (see *note Processing options::). If this option is given a value of zero or one, no smoothing will be done. Without smoothing, strong boundaries will probably be created between the values estimated for each tile. It is thus good to smooth the interpolated image so strong discontinuities do not show up in the final Sky values. The smoothing is done through convolution (see *note Convolution process::) with a flat kernel, so the value to this option must be an odd number. ‘--checksky’ Create a multi-extension FITS file showing the steps that were used to estimate the Sky value over the input, see *note Quantifying signal in a tile::. The file will have two extensions for each step (one for the Sky and one for the Sky standard deviation). ---------- Footnotes ---------- (1) You can try it by running the command in the ‘tests’ directory, open the image with a FITS viewer and have a look at it to get a sense of how these statistics relate to the input image/dataset. (2) gnuastro-0.5/doc/gnuastro.info-10000644000175000017500000111407413217220434013571 00000000000000This is gnuastro.info, produced by makeinfo version 6.5 from gnuastro.texi. This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro’s library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. END-INFO-DIR-ENTRY  File: gnuastro.info, Node: Top, Next: Introduction, Prev: (dir), Up: (dir) GNU Astronomy Utilities *********************** This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. * Menu: * Introduction:: General introduction. * Tutorials:: Tutorials or Cookbooks. * Installation:: Requirements and installation. * Common program behavior:: Common behavior in all programs. * Data containers:: Tools to operate on extensions and tables. * Data manipulation:: Tools for basic image manipulation. * Data analysis:: Analyze images. * Modeling and fittings:: Make and fit models. * High-level calculations:: Physical calculations. * Library:: Gnuastro’s library of useful functions. * Developing:: The development environment. * Gnuastro programs list:: List and short summary of Gnuastro. * Other useful software:: Installing other useful software. * GNU Free Doc. License:: GNU Free documentation license. * Index:: Index of terms — The Detailed Node Listing — Introduction * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production. Version numbering * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release New to GNU/Linux? * Command-line interface:: Introduction to the command-line Tutorials * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. * General program usage tutorial:: Usage of all programs in a good way. Installation * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. Dependencies * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source. Mandatory dependencies * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS. Downloading the source * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source. Version controlled source * Bootstrapping:: Adding all the automatically generated files. * Synchronizing:: Keep your local clone up to date. Build and install * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter. Configuring * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source. Common program behavior * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Multi-threaded operations:: How threads are managed in Gnuastro. * Numeric data types:: Different types and how to specify them. * Tables:: Recognized table formats. * Tessellation:: Tile the dataset into non-overlapping bins. * Getting help:: Getting more information on the go. * Automatic output:: About automatic output names. * Output headers:: Common headers to all FITS outputs. Command-line * Arguments and options:: Basics of options and arguments. * Common options:: Common options to all Gnuastro programs. Arguments and options * Arguments:: For specifying the main input files/operations. * Options:: For configuring the behavior of the program. Common options * Input output options:: Common input/output options. * Processing options:: Options for common processing steps. * Operating mode options:: Common operating mode options. Configuration files * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. Multi-threaded operations * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously. Tables * Recognized table formats:: Table formats that are recognized in Gnuastro. * Gnuastro text table format:: Gnuastro’s convention plain text tables. * Selecting table columns:: Identify/select certain columns from a table Recognized table formats * Gnuastro text table format:: Reading plain text tables Getting help * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from –help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users. Data containers * Fits:: View and manipulate extensions and keywords. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text. Fits * Invoking astfits:: Arguments and options to Header. Invoking Fits * HDU manipulation:: Manipulate HDUs within a FITS file. * Keyword manipulation:: Manipulate metadata keywords in a HDU ConvertType * Recognized file formats:: Recognized file formats * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType. Table * Invoking asttable:: Options and arguments to Table. Data manipulation * Crop:: Crop region(s) from a dataset. * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * Warp:: Warp/Transform an image to a different grid. Crop * Crop modes:: Basic modes to define crop region. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astcrop:: Calling Crop on the command-line Invoking Crop * Crop options:: A list of all the options with explanation. * Crop output:: The outputs of Crop. Arithmetic * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output Convolve * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. Spatial domain convolution * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. Frequency domain and Fourier operations * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects. Warp * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astwarp:: Arguments and options for Warp. Data analysis * Statistics:: Calculate dataset statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. * Match:: Match two datasets. Statistics * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of $\sigma$-clipping. * Sky value:: Definition and derivation of the Sky value. * Invoking aststatistics:: Arguments and options to Statistics. Sky value * Sky value definition:: Definition of the Sky/reference value. * Sky value misconceptions:: Wrong methods to estimate the Sky value. * Quantifying signal in a tile:: Method to estimate the presence of signal. NoiseChisel * NoiseChisel changes after publication:: Changes to the software after publication. * Invoking astnoisechisel:: Options and arguments for NoiseChisel. Invoking NoiseChisel * General NoiseChisel options:: General NoiseChisel preprocessing. * Detection options:: Configure detection in NoiseChisel. * Segmentation options:: Configure segmentation in NoiseChisel. * NoiseChisel output:: NoiseChisel’s output format. MakeCatalog * Detection and catalog production:: Discussing why/how to treat these separately * Quantifying measurement limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Adding new columns to MakeCatalog:: How to add new columns. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. Invoking MakeCatalog * MakeCatalog input files:: Specifying the different input files. * MakeCatalog general settings:: Options for general column settings. * Upper-limit magnitude settings:: Necessary to define upper-limit magnitudes. * MakeCatalog output columns:: How to specify the columns in the output. Match * Invoking astmatch:: Inputs, outputs and options of Match Modeling and fitting * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image. MakeProfiles * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles. Modeling basics * Defining an ellipse:: An ellipse on a pixelated grid. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model. Invoking MakeProfiles * MakeProfiles catalog:: Required catalog properties. * MakeProfiles profile settings:: Configuration parameters for all profiles. * MakeProfiles output dataset:: The canvas/dataset to build profiles over. * MakeProfiles log file:: A description of the optional log file. MakeNoise * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. Noise basics * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated. High-level calculations * CosmicCalculator:: Calculate cosmological variables CosmicCalculator * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator Invoking CosmicCalculator * CosmicCalculator input options:: Options to specify input conditions. * CosmicCalculator specific calculations:: Requesting specific outputs. Library * Review of library fundamentals:: Guide on libraries and linking. * BuildProgram:: Link and run source files with this library. * Gnuastro library:: Description of all library functions. * Library demo programs:: Demonstration for using libraries. Review of library fundamentals * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. BuildProgram * Invoking astbuildprog:: Options and examples for using this program. Gnuastro library * Configuration information:: General information about library config. * Multithreaded programming:: Tools for easy multi-threaded operations. * Library data types:: Definitions and functions for types. * Library blank values:: Blank values and functions to deal with them. * Library data container:: General data container in Gnuastro. * Dimensions:: Dealing with coordinates and dimensions. * Linked lists:: Various types of linked lists. * FITS files:: Working with FITS data. * World Coordinate System:: Dealing with the world coordinate system. * Text files:: Functions to work on Text files. * Table input output:: Reading and writing table columns. * Arithmetic on datasets:: Arithmetic operations on a dataset. * Tessellation library:: Functions for working on tiles. * Bounding box:: Finding the bounding box. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Permutations:: Re-order (or permute) the values in a dataset. * Matching:: Matching catalogs based on position. * Statistical operations:: Functions for basic statistics. * Binary datasets:: Datasets that can only have values of 0 or 1. * Convolution functions:: Library functions to do convolution. * Interpolation:: Interpolate (over blank values possibly). * Git wrappers:: Wrappers for functions in libgit2. * Cosmology library:: Cosmological calculations. Multithreaded programming (‘threads.h’) * Implementation of pthread_barrier:: Some systems don’t have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. Data container (‘data.h’) * Generic data container:: Definition of Gnuastro’s generic container. * Dataset size and allocation:: Functions for size and allocation. * Arrays of datasets:: Functions to help with array of datasets. * Copying datasets:: Functions to copy a dataset to a new one. Linked lists (‘list.h’) * List of strings:: Simply linked list of strings. * List of int32_t:: Simply linked list of int32_ts. * List of size_t:: Simply linked list of size_ts. * List of float:: Simply linked list of floats. * List of double:: Simply linked list of doubles * List of void:: Simply linked list of void * pointers. * Ordered list of size_t:: Simply linked, ordered list of size_t. * Doubly linked ordered list of size_t:: Definition and functions. * List of gal_data_t:: Simply linked list Gnuastro’s generic datatype. FITS files (‘fits.h’) * FITS macros errors filenames:: General macros, errors and checking names. * CFITSIO and Gnuastro types:: Conversion between FITS and Gnuastro types. * FITS HDUs:: Opening and getting information about HDUs. * FITS header keywords:: Reading and writing FITS header keywords. * FITS arrays:: Reading and writing FITS images/arrays. * FITS tables:: Reading and writing FITS tables. Tessellation library (‘tile.h’) * Independent tiles:: Work on or check independent tiles. * Tile grid:: Cover a full dataset with non-overlapping tiles. Library demo programs * Library demo - reading a image:: Read a FITS image into memory. * Library demo - inspecting neighbors:: Inspect the neighbors of a pixel. * Library demo - multi-threaded operation:: Doing an operation on threads. * Library demo - reading and writing table columns:: Simple Column I/O. Developing * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro’s development. * Contributing to Gnuastro:: Share your changes with all users. Program source * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program. Contributing to Gnuastro * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git. Other useful software * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C SAO ds9 * Viewing multiextension FITS images:: Configure SAO ds9 for multiextension images.  File: gnuastro.info, Node: Introduction, Next: Tutorials, Prev: Top, Up: Top 1 Introduction ************** GNU Astronomy Utilities (Gnuastro) is an official GNU package consisting of separate programs and libraries for the manipulation and analysis of astronomical data. All the programs share the same basic command-line user interface for the comfort of both the users and developers. Gnuastro is written to comply fully with the GNU coding standards so it integrates finely with the GNU/Linux operating system. This also enables astronomers to expect a fully familiar experience in the source code, building, installing and command-line user interaction that they have seen in all the other GNU software that they use. The official and always up to date version of this book (or manual) is freely available under *note GNU Free Doc. License:: in various formats (pdf, html, plain text, info, and as its Texinfo source) at . For users who are new to the GNU/Linux environment, unless otherwise specified most of the topics in *note Installation:: and *note Common program behavior:: are common to all GNU software, for example installation, managing command-line options or getting help (also see *note New to GNU/Linux?::). So if you are new to this empowering environment, we encourage you to go through these chapters carefully. They can be a starting point from which you can continue to learn more from each program’s own manual and fully benefit from and enjoy this wonderful environment. Gnuastro also comes with a large set of libraries, so you can write your own programs using Gnuastro’s building blocks, see *note Review of library fundamentals:: for an introduction. Finally it must be mentioned that in Gnuastro, no change to any program will be released before it has been fully documented in this here first. As discussed in *note Science and its tools:: this is the founding basis of the Gnuastro. * Menu: * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production.  File: gnuastro.info, Node: Quick start, Next: Science and its tools, Prev: Introduction, Up: Introduction 1.1 Quick start =============== The latest official release tarball is always available as ‘gnuastro-latest.tar.gz’ (http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.gz). For better compression (faster download), and robust archival features, an Lzip (http://www.nongnu.org/lzip/lzip.html) compressed tarball is also available at ‘gnuastro-latest.tar.lz’ (http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.lz), see *note Release tarball:: for more details on the tarball release. The Gzip library and program are commonly available on most systems. However, Gnuastro recommends Lzip as described above and the beta-releases are also only distributed in ‘tar.lz’. You can download and install Lzip’s source (in ‘.tar.gz’ format) from its webpage and follow the same process as below: Lzip has no dependencies, so simply decompress, then run ‘./configure’, ‘make’, ‘sudo make install’. Let’s assume the downloaded tarball is in the ‘TOPGNUASTRO’ directory. The first two commands below can be used to decompress the source. If you download ‘tar.lz’ and your Tar implementation doesn’t recognize Lzip (the second command fails), run the third and fourth lines. Note that lines starting with ‘##’ don’t need to be typed. ## Go into the download directory. $ cd TOPGNUASTRO ## Also works on `tar.gz'. GNU Tar recognizes both formats. $ tar xf gnuastro-latest.tar.lz ## Only when previous command fails. $ lzip -d gnuastro-latest.tar.lz $ tar xf gnuastro-latest.tar Gnuastro has three mandatory dependencies and some optional dependencies for extra functionality, see *note Dependencies:: for the full list. Links to the dependency sources and instructions on installing each are fully described there. When the mandatory dependencies are ready, you can configure, compile, check and install Gnuastro on your system with the following commands. $ cd gnuastro-X.X # Replace X.X with version number. $ ./configure $ make -j8 # Replace 8 with no. CPU threads. $ make check $ sudo make install See *note Known issues:: if you confront any complications. For each program there is an ‘Invoke ProgramName’ sub-section in this book which explains how the programs should be run on the command-line (for example *note Invoking asttable::). You can read the same section on the command-line by running ‘$ info astprogname’ (for example ‘info asttable’). The ‘Invoke ProgramName’ sub-section starts with a few examples of each program and goes on to explain the invocation details. See *note Getting help:: for all the options you have to get help. In *note Tutorials:: some real life examples of how these programs might be used are given.  File: gnuastro.info, Node: Science and its tools, Next: Your rights, Prev: Quick start, Up: Introduction 1.2 Science and its tools ========================= History of science indicates that there are always inevitably unseen faults, hidden assumptions, simplifications and approximations in all our theoretical models, data acquisition and analysis techniques. It is precisely these that will ultimately allow future generations to advance the existing experimental and theoretical knowledge through their new solutions and corrections. In the past, scientists would gather data and process them individually to achieve an analysis thus having a much more intricate knowledge of the data and analysis. The theoretical models also required little (if any) simulations to compare with the data. Today both methods are becoming increasingly more dependent on pre-written software. Scientists are dissociating themselves from the intricacies of reducing raw observational data in experimentation or from bringing the theoretical models to life in simulations. These ‘intricacies’ are precisely those unseen faults, hidden assumptions, simplifications and approximations that define scientific progress. Unfortunately, most persons who have recourse to a computer for statistical analysis of data are not much interested either in computer programming or in statistical method, being primarily concerned with their own proper business. Hence the common use of library programs and various statistical packages. ... It’s time that was changed. — _F. J. Anscombe. The American Statistician, Vol. 27, No. 1. 1973_ Anscombe’s quartet (http://en.wikipedia.org/wiki/Anscombe%27s_quartet) demonstrates how four data sets with widely different shapes (when plotted) give nearly identical output from standard regression techniques. Anscombe uses this (now famous) quartet, which was introduced in the paper quoted above, to argue that “Good statistical analysis is not a purely routine matter, and generally calls for more than one pass through the computerâ€. Anscombe’s quartet can be generalized to say that users of a software cannot claim to understand how it works only based on the experience they have gained by frequently using it. This kind of subjective experience is prone to very serious mis-understandings about the data, what the software/statistical-method really does (especially as it gets more complicated), and thus the scientific interpretation of the result. This attitude is further encouraged through non-free software(1). This approach to scientific software only helps in producing dogmas and an “obscurantist faith in the expert’s special skill, and in his personal knowledge and authorityâ€(2). Program or be programmed. Choose the former, and you gain access to the control panel of civilization. Choose the latter, and it could be the last real choice you get to make. — _Douglas Rushkoff. Program or be programmed, O/R Books (2010)._ It is obviously impractical for any one human being to gain the intricate knowledge explained above for every step of an analysis. On the other hand, scientific data can be very large and numerous, for example images produced by telescopes in astronomy. This requires very efficient algorithms. To make things worse, natural scientists have generally not been trained in the advanced software techniques, paradigms and architecture that are taught in computer science or engineering courses and thus used in most software. The GNU Astronomy Utilities are an effort to tackle this issue. Gnuastro is not just a software, this book is as important to the idea behind Gnuastro as the source code (software). This book has tried to learn from the success of the “Numerical Recipes†book in educating those who are not software engineers and computer scientists but still heavy users of computational algorithms, like astronomers. There are two major differences: the code and the explanations are segregated: the code is moved within the actual Gnuastro software source code and the underlying explanations are given here. In the source code every non-trivial step is heavily commented and correlated with this book, it follows the same logic of this book, and all the programs follow a similar internal data, function and file structure, see *note Program source::. Complementing the code, this book focuses on thoroughly explaining the concepts behind those codes (history, mathematics, science, software and usage advise when necessary) along with detailed instructions on how to run the programs. At the expense of frustrating “professionals†or “expertsâ€, this book and the comments in the code also intentionally avoid jargon and abbreviations. The source code and this book are thus intimately linked, and when considered as a single entity can be thought of as a real (an actual software accompanying the algorithms) “Numerical Recipes†for astronomy. The other major and arguably more important difference is that “Numerical Recipes†does not allow you to distribute any code that you have learned from it. So while it empowers the privileged individual who has access to it, it exacerbates social ignorance. For example it does not allow you to release your software’s source code if you have used their codes, you can only publicly release binaries (a black box) to the community. Exactly at the opposite end of the spectrum, Gnuastro’s source code is released under the GNU general public license (GPL) and this book is released under the GNU free documentation license. You are therefore free to distribute any software you create using parts of Gnuastro’s source code or text, or figures from this book, see *note Your rights::. While developing the source code and this book together, the developers of Gnuastro aim to impose the minimum requirements on you (in computer science, engineering and even the mathematics behind the tools) to understand and modify any step of Gnuastro if you feel the need to do so, see *note Why C:: and *note Program design philosophy::. Imagine if Galileo did not have the technical knowledge to build a telescope. Astronomical objects could not be seen with the Dutch military design of the telescope. In the beginning of his “The Sidereal Messenger†(1610) he cautions the readers on this issue and instructs them on how to build a suitable instrument: without a detailed description of “how†he made his observations, no one would believe him. The same is true today, science cannot progress with a black box. Before he actually saw the moons of Jupiter, the mountains on the Moon or the crescent of Venus, he was “evasive†to Kepler(3). Science is not independent of its tools. Bjarne Stroustrup (creator of the C++ language) says: “Without understanding software, you are reduced to believing in magicâ€. Ken Thomson (the designer or the Unix operating system) says “I abhor a system designed for the ‘user’ if that word is a coded pejorative meaning ‘stupid and unsophisticated’.†Certainly no scientist (user of a scientific software) would want to be considered a believer in magic, or ‘stupid and unsophisticated’. However, this can happen when scientists get too distant from the raw data and are mainly indulging themselves in their own high-level (abstract) models (creations). For example, roughly five years before special relativity and about two decades before quantum mechanics fundamentally changed Physics, Kelvin is quoted as saying: There is nothing new to be discovered in physics now. All that remains is more and more precise measurement. — _William Thomson (Lord Kelvin), 1900_ A few years earlier, in a speech Albert. A. Michelson said: The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decimals. — _Albert. A. Michelson, dedication of Ryerson Physics Lab, U. Chicago 1894_ If scientists are considered to be more than mere “puzzle solversâ€(4) (simply adding to the decimals of known values or observing a feature in 10, 100, or 100000 more galaxies or stars, as Kelvin and Michelson clearly believed), they cannot just passively sit back and uncritically repeat the previous (observational or theoretical) methods/tools on new data. Today there is a wealth of raw telescope images ready (mostly for free) at the finger tips of anyone who is interested with a fast enough internet connection to download them. The only thing lacking is new ways to analyze this data and dig out the treasure that is lying hidden in them to existing methods and techniques. New data that we insist on analyzing in terms of old ideas (that is, old models which are not questioned) cannot lead us out of the old ideas. However many data we record and analyze, we may just keep repeating the same old errors, missing the same crucially important things that the experiment was competent to find. — _Jaynes, Probability theory, the logic of science. Cambridge U. Press (2003)._ ---------- Footnotes ---------- (1) (2) Karl Popper. The logic of scientific discovery. 1959. Larger quote is given at the start of the PDF (for print) version of this book. (3) Galileo G. (Translated by Maurice A. Finocchiaro). _The essential Galileo_. Hackett publishing company, first edition, 2008. (4) Thomas S. Kuhn. _The Structure of Scientific Revolutions_, University of Chicago Press, 1962.  File: gnuastro.info, Node: Your rights, Next: Naming convention, Prev: Science and its tools, Up: Introduction 1.3 Your rights =============== The paragraphs below, in this section, belong to the GNU Texinfo(1) manual and are not written by us! The name “Texinfo†is just changed to “GNU Astronomy Utilities†or “Gnuastro†because they are released under the same licenses and it is beautifully written to inform you of your rights. GNU Astronomy Utilities is “free softwareâ€; this means that everyone is free to use it and free to redistribute it on certain conditions. Gnuastro is not in the public domain; it is copyrighted and there are restrictions on its distribution, but these restrictions are designed to permit everything that a good cooperating citizen would want to do. What is not allowed is to try to prevent others from further sharing any version of Gnuastro that they might get from you. Specifically, we want to make sure that you have the right to give away copies of the programs that relate to Gnuastro, that you receive the source code or else can get it if you want it, that you can change these programs or use pieces of them in new free programs, and that you know you can do these things. To make sure that everyone has such rights, we have to forbid you to deprive anyone else of these rights. For example, if you distribute copies of the Gnuastro related programs, you must give the recipients all the rights that you have. You must make sure that they, too, receive or can get the source code. And you must tell them their rights. Also, for our own protection, we must make certain that everyone finds out that there is no warranty for the programs that relate to Gnuastro. If these programs are modified by someone else and passed on, we want their recipients to know that what they have is not what we distributed, so that any problems introduced by others will not reflect on our reputation. The precise conditions of the licenses for the programs currently being distributed that relate to Gnuastro are found in the GNU General Public license (http://www.gnu.org/copyleft/gpl.html) that accompany them. This book is covered by the GNU Free Documentation License (http://www.gnu.org/copyleft/fdl.html). ---------- Footnotes ---------- (1) Texinfo is the GNU documentation system. It is used to create this book in all the various formats.  File: gnuastro.info, Node: Naming convention, Next: Version numbering, Prev: Your rights, Up: Introduction 1.4 Naming convention ===================== Gnuastro is a package of independent programs and a collection of libraries, here we are mainly concerned with the programs. Each program has an official name which consists of one or two words, describing what they do. The latter are printed with no space, for example NoiseChisel or Crop. On the command-line, you can run them with their executable names which start with an ‘ast’ and might be an abbreviation of the official name, for example ‘astnoisechisel’ or ‘astcrop’, see *note Executable names::. We will use “ProgramName†for a generic official program name and ‘astprogname’ for a generic executable name. In this book, the programs are classified based on what they do and thoroughly explained. An alphabetical list of the programs that are installed on your system with this installation are given in *note Gnuastro programs list::. That list also contains the executable names and version numbers along with a one line description.  File: gnuastro.info, Node: Version numbering, Next: New to GNU/Linux?, Prev: Naming convention, Up: Introduction 1.5 Version numbering ===================== Gnuastro can have two formats of version numbers, for official and unofficial releases. Official Gnuastro releases are announced on the ‘info-gnuastro’ mailing list, they have a version control tag in Gnuastro’s development history, and their version numbers are formatted like “‘A.B’â€. ‘A’ is a major version number, marking a significant planned achievement (for example see *note GNU Astronomy Utilities 1.0::), while ‘B’ is a minor version number, see below for more on the distinction. Note that the numbers are not decimals, so version 2.34 is much more recent than version 2.5, which is not equal to 2.50. Gnuastro also allows a unique version number for unofficial releases. Unofficial releases can mark any point in Gnuastro’s development history. This is done to allow astronomers to easily use any point in the version controlled history for their data-analysis and research publication. See *note Version controlled source:: for a complete introduction. This section is not just for developers and is very straightforward, so please have a look if you are interested in the cutting-edge. This unofficial version number is a meaningful and easy to read string of characters, unique to that particular point of history. With this feature, users can easily stay up to date with the most recent bug fixes and additions that are committed between official releases. The unofficial version number is formatted like: ‘A.B.C-D’. ‘A’ and ‘B’ are the most recent official version number. ‘C’ is the number of commits that have been made after version ‘A.B’. ‘D’ is the first 4 or 5 characters of the commit hash number(1). Therefore, the unofficial version number ‘‘3.92.8-29c8’’, corresponds to the 8th commit after the official version ‘3.92’ and its commit hash begins with ‘29c8’. The unofficial version number is sort-able (unlike the raw hash) and as shown above is very descriptive of the state of the unofficial release. Of course an official release is preferred for publication (since its tarballs are easily available and it has gone through more tests, making it more stable), so if an official release is announced prior to your publication’s final review, please consider updating to the official release. The major version number is set by a major goal which is defined by the developers and user community before hand, for example see *note GNU Astronomy Utilities 1.0::. The incremental work done in minor releases are commonly small steps in achieving the major goal. Therefore, there is no limit on the number of minor releases and the difference between the (hypothetical) versions 2.927 and 3.0 can be a very small (negligible to the user) improvement that finalizes the defined goals. * Menu: * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release ---------- Footnotes ---------- (1) Each point in Gnuastro’s history is uniquely identified with a 40 character long hash which is created from its contents and previous history for example: ‘5b17501d8f29ba3cd610673261e6e2229c846d35’. So the string ‘D’ in the version for this commit could be ‘5b17’, or ‘5b175’.  File: gnuastro.info, Node: GNU Astronomy Utilities 1.0, Prev: Version numbering, Up: Version numbering 1.5.1 GNU Astronomy Utilities 1.0 --------------------------------- Currently (prior to Gnuastro 1.0), the aim of Gnuastro is to have a complete system for data manipulation and analysis at least similar to IRAF(1). So an astronomer can take all the standard data analysis steps (starting from raw data to the final reduced product and standard post-reduction tools) with the various programs in Gnuastro. The maintainers of each camera or detector on a telescope can provide a completely transparent shell script or Makefile to the observer for data analysis. This script can set configuration files for all the required programs to work with that particular camera. The script can then run the proper programs in the proper sequence. The user/observer can easily follow the standard shell script to understand (and modify) each step and the parameters used easily. Bash (or other modern GNU/Linux shell scripts) are very powerful and made for this gluing job. This will simultaneously improve performance and transparency. Shell scripting (or Makefiles) are also very basic constructs that are easy to learn and readily available as part of the Unix-like operating systems. If there is no program to do a desired step, Gnuastro’s libraries can be used to build specific programs. The main factor is that all observatories or projects can freely contribute to Gnuastro and all simultaneously benefit from it (since it doesn’t belong to any particular one of them), much like how for-profit organizations (for example RedHat, or Intel and many others) are major contributors to free and open source software for their shared benefit. Gnuastro’s copyright has been fully awarded to GNU, so it doesn’t belong to any particular astronomer or astronomical facility or project. ---------- Footnotes ---------- (1)  File: gnuastro.info, Node: New to GNU/Linux?, Next: Report a bug, Prev: Version numbering, Up: Introduction 1.6 New to GNU/Linux? ===================== Some astronomers initially install and use the GNU/Linux operating systems because the software that their research community use can only be run in this environment, the transition is not necessarily easy. To encourage you in investing the patience and time to make this transition, we define the GNU/Linux system and argue for the command-line interface of scientific software and how it is worth the (apparently steep) learning curve. *note Command-line interface:: contains a short overview of the very powerful command-line user interface. *note Tutorials:: is a complete chapter with some real world example applications of Gnuastro making good use of GNU/Linux capabilities written for newcomers to this environment. It is fully explained, easy and (hopefully) entertaining. You might have already noticed that we are not using the name “Linuxâ€, but “GNU/Linuxâ€. Please take the time to have a look at the following essays and FAQs for a complete understanding of this very important distinction. In short, the Linux kernel is built using the GNU C library (glibc) and GNU compiler collection (gcc). The Linux kernel software alone is useless, in order have an operating system you need many more packages and the majority of such low-level packages in most distributions are developed as part of the GNU project: “the whole system is basically GNU with Linux loadedâ€. In the form of an analogy: to say “running Linuxâ€, is like saying “driving your carburetorâ€. • • • • * Menu: * Command-line interface:: Introduction to the command-line  File: gnuastro.info, Node: Command-line interface, Prev: New to GNU/Linux?, Up: New to GNU/Linux? 1.6.1 Command-line interface ---------------------------- One aspect of Gnuastro that might be a little troubling to new GNU/Linux users is that (at least for the time being) it only has a command-line user interface (CLI). This might be contrary to the mostly graphical user interface (GUI) experience with proprietary operating systems. To a first time user, the command-line does appear much more complicated and adapting to it might not be easy and a little frustrating at first. This is understandable and also experienced by anyone who started using the computer (from childhood) in a graphical user interface. Here we hope to convince you of the unique benefits of this interface which can greatly enhance your productivity while complementing your GUI experience. Through GNOME 3(1), most GNU/Linux based operating systems now have a very advanced and useful GUI. Since the GUI was created long after the command-line, some wrongly consider the command line to be obsolete. Both interfaces are very useful for different tasks (for example you can’t view an image, video, pdf document or web page on the command-line!), on the other hand you can’t reproduce your results easily in the GUI. Therefore they should not be regarded as rivals but as complementary user interfaces, here we will outline how the CLI can be useful in scientific programs. You can think of the GUI as a veneer over the CLI to facilitate a small subset of all the possible CLI operations. Each click you do on the GUI, can be thought of as internally running a different CLI command. So asymptotically (if a good designer can design a GUI which is able to show you all the possibilities to click on) the GUI is only as powerful as the command-line. In practice, such graphical designers are very hard to find for every program, so the GUI operations are always a subset of the internal CLI commands. For programs that are only made for the GUI, this results in not including lots of potentially useful operations. It also results in ‘interface design’ to be a crucially important part of any GUI program. Scientists don’t usually have enough resources to hire a graphical designer, also the complexity of the GUI code is far more than CLI code, which is harmful for a scientific software, see *note Science and its tools::. For programs that have a GUI, one action on the GUI (moving and clicking a mouse, or tapping a touchscreen) might be more efficient and easier than its CLI counterpart (typing the program name and your desired configuration). However, if you have to repeat that same action more than once, the GUI will soon become very frustrating and prone to errors. Unless the designers of a particular program decided to design such a system for a particular GUI action, there is no general way to run any possible series of actions automatically on the GUI. On the command-line, you can run any series of of actions which can come from various CLI capable programs you have decided your self in any possible permutation with one command(2). This allows for much more creativity and exact reproducibility that is not possible to a GUI user. For technical and scientific operations, where the same operation (using various programs) has to be done on a large set of data files, this is crucially important. It also allows exact reproducibility which is a foundation principle for scientific results. The most common CLI (which is also known as a shell) in GNU/Linux is GNU Bash, we strongly encourage you to put aside several hours and go through this beautifully explained web page: . You don’t need to read or even fully understand the whole thing, only a general knowledge of the first few chapters are enough to get you going. Since the operations in the GUI are very limited and they are visible, reading a manual is not that important in the GUI (most programs don’t even have any!). However, to give you the creative power explained above, with a CLI program, it is best if you first read the manual of any program you are using. You don’t need to memorize any details, only an understanding of the generalities is needed. Once you start working, there are more easier ways to remember a particular option or operation detail, see *note Getting help::. To experience the command-line in its full glory and not in the GUI terminal emulator, press the following keys together: (3) to access the virtual console. To return back to your GUI, press the same keys above replacing with (or , or , depending on your GNU/Linux distribution). In the virtual console, the GUI, with all its distracting colors and information, is gone. Enabling you to focus entirely on your actual work. For operations that use a lot of your system’s resources (processing a large number of large astronomical images for example), the virtual console is the place to run them. This is because the GUI is not competing with your research work for your system’s RAM and CPU. Since the virtual consoles are completely independent, you can even log out of your GUI environment to give even more of your hardware resources to the programs you are running and thus reduce the operating time. Since it uses far less system resources, the CLI is also very convenient for remote access to your computer. Using secure shell (SSH) you can log in securely to your system (similar to the virtual console) from anywhere even if the connection speeds are low. There are apps for smart phones and tablets which allow you to do this. ---------- Footnotes ---------- (1) (2) By writing a shell script and running it, for example see the tutorials in *note Tutorials::. (3) Instead of , you can use any of the keys from to for different virtual consoles depending on your GNU/Linux distribution, try them all out. You can also run a separate GUI from within this console if you want to.  File: gnuastro.info, Node: Report a bug, Next: Suggest new feature, Prev: New to GNU/Linux?, Up: Introduction 1.7 Report a bug ================ According to Wikipedia “a software bug is an error, flaw, failure, or fault in a computer program or system that causes it to produce an incorrect or unexpected result, or to behave in unintended waysâ€. So when you see that a program is crashing, not reading your input correctly, giving the wrong results, or not writing your output correctly, you have found a bug. In such cases, it is best if you report the bug to the developers. The programs will also report bugs in known impossible situations (which are caused by something unexpected) and will ask the users to report the bug. Prior to actually filing a bug report, it is best to search previous reports. The issue might have already been found and even solved. The best place to check if your bug has already been discussed is the bugs tracker on *note Gnuastro project webpage:: at . In the top search fields (under “Display Criteriaâ€) set the “Open/Closed†drop-down menu to “Any†and choose the respective program or general category of the bug in “Category†and click the “Apply†button. The results colored green have already been solved and the status of those colored in red is shown in the table. Recently corrected bugs are probably not yet publicly released because they are scheduled for the next Gnuastro stable release. If the bug is solved but not yet released and it is an urgent issue for you, you can get the version controlled source and compile that, see *note Version controlled source::. To solve the issue as readily as possible, please follow the following to guidelines in your bug report. The How to Report Bugs Effectively (http://www.chiark.greenend.org.uk/~sgtatham/bugs.html) and How To Ask Questions The Smart Way (http://catb.org/~esr/faqs/smart-questions.html) essays also provide some very good generic advice for all software (don’t contact their authors for Gnuastro’s problems). Mastering the art of giving good bug reports (like asking good questions) can greatly enhance your experience with any free and open source software. So investing the time to read through these essays will greatly reduce your frustration after you see something doesn’t work the way you feel it is supposed to for a large range of software, not just Gnuastro. *Be descriptive* Please provide as many details as possible and be very descriptive. Explain what you expected and what the output was: it might be that your expectation was wrong. Also please clearly state which sections of the Gnuastro book (this book), or other references you have studied to understand the problem. This can be useful in correcting the book (adding links to likely places where users will check). But more importantly, it will be very encouraging for the developers, since you are showing how serious you are about the problem and that you have actually put some thought into it. “To be able to ask a question clearly is two-thirds of the way to getting it answered.†– John Ruskin (1819-1900). *Individual and independent bug reports* If you have found multiple bugs, please send them as separate (and independent) bugs (as much as possible). This will significantly help us in managing and resolving them sooner. *Reproducible bug reports* If we cannot exactly reproduce your bug, then it is very hard to resolve it. So please send us a Minimal working example(1) along with the description. For example in running a program, please send us the full command-line text and the output with the ‘-P’ option, see *note Operating mode options::. If it is caused only for a certain input, also send us that input file. In case the input FITS is large, please use Crop to only crop the problematic section and make it as small as possible so it can easily be uploaded and downloaded and not waste the archive’s storage, see *note Crop::. There are generally two ways to inform us of bugs: • Send a mail to ‘bug-gnuastro@gnu.org’. Any mail you send to this address will be distributed through the bug-gnuastro mailing list(2). This is the simplest way to send us bug reports. The developers will then register the bug into the project webpage (next choice) for you. • Use the Gnuastro project webpage at : There are two ways to get to the submission page as listed below. Fill in the form as described below and submit it (see *note Gnuastro project webpage:: for more on the project webpage). • Using the top horizontal menu items, immediately under the top page title. Hovering your mouse on “Support†will open a drop-down list. Select “Submit newâ€. • In the main body of the page, under the “Communication tools†section, click on “Submit new itemâ€. Once the items have been registered in the mailing list or webpage, the developers will add it to either the “Bug Tracker†or “Task Manager†trackers of the Gnuastro project webpage. These two trackers can only be edited by the Gnuastro project developers, but they can be browsed by anyone, so you can follow the progress on your bug. You are most welcome to join us in developing Gnuastro and fixing the bug you have found maybe a good starting point. Gnuastro is designed to be easy for anyone to develop (see *note Science and its tools::) and there is a full chapter devoted to developing it: *note Developing::. ---------- Footnotes ---------- (1) (2)  File: gnuastro.info, Node: Suggest new feature, Next: Announcements, Prev: Report a bug, Up: Introduction 1.8 Suggest new feature ======================= We would always be very happy to hear of suggested new features. For every program there are already lists of features that we are planning to add. You can see the current list of plans from the Gnuastro project webpage at and following “Tasksâ€â†’“Browse†on the horizontal menu at the top of the page immediately under the title, see *note Gnuastro project webpage::. If you want to request a feature to an existing program, click on the “Display Criteria†above the list and under “Categoryâ€, choose that particular program. Under “Category†you can also see the existing suggestions for new programs or other cases like installation, documentation or libraries. Also be sure to set the “Open/Closed†value to “Anyâ€. If the feature you want to suggest is not already listed in the task manager, then follow the steps that are fully described in *note Report a bug::. Please have in mind that the developers are all very busy with their own astronomical research, and implementing existing “taskâ€s to add or resolving bugs. Gnuastro is a volunteer effort and none of the developers are paid for their hard work. So, although we will try our best, please don’t not expect that your suggested feature be immediately included (with the next release of Gnuastro). The best person to apply the exciting new feature you have in mind is you, since you have the motivation and need. In fact Gnuastro is designed for making it as easy as possible for you to hack into it (add new features, change existing ones and so on), see *note Science and its tools::. Please have a look at the chapter devoted to developing (*note Developing::) and start applying your desired feature. Once you have added it, you can use it for your own work and if you feel you want others to benefit from your work, you can request for it to become part of Gnuastro. You can then join the developers and start maintaining your own part of Gnuastro. If you choose to take this path of action please contact us before hand (*note Report a bug::) so we can avoid possible duplicate activities and get interested people in contact. *Gnuastro is a collection of low level programs:* As described in *note Program design philosophy::, a founding principle of Gnuastro is that each library or program should be very basic and low-level. High level jobs should be done by running the separate programs or using separate functions in succession through a shell script or calling the libraries by higher level functions, see the examples in *note Tutorials::. So when making the suggestions please consider how your desired job can best be broken into separate steps and modularized.  File: gnuastro.info, Node: Announcements, Next: Conventions, Prev: Suggest new feature, Up: Introduction 1.9 Announcements ================= Gnuastro has a dedicated mailing list for making announcements. Anyone that is interested can subscribe to this mailing list to stay up to date with new releases or when the dependencies (see *note Dependencies::) have been updated. To subscribe to this list, please visit .  File: gnuastro.info, Node: Conventions, Next: Acknowledgments, Prev: Announcements, Up: Introduction 1.10 Conventions ================ In this book we have the following conventions: • All commands that are to be run on the shell (command-line) prompt as the user start with a ‘$’. In case they must be run as a super-user or system administrator, they will start with a single ‘#’. If the command is in a separate line and next line ‘is also in the code type face’, but doesn’t have any of the ‘$’ or ‘#’ signs, then it is the output of the command after it is run. As a user, you don’t need to type those lines. A line that starts with ‘##’ is just a comment for explaining the command to a human reader and must not be typed. • If the command becomes larger than the page width a <\> is inserted in the code. If you are typing the code by hand on the command-line, you don’t need to use multiple lines or add the extra space characters, so you can omit them. If you want to copy and paste these examples (highly discouraged!) then the <\> should stay. The <\> character is a shell escape character which is used commonly to make characters which have special meaning for the shell loose that special place (the shell will not treat them specially if there is a <\> behind them). When it is a last character in a line (the next character is a new-line character) the new-line character looses its meaning an the shell sees it as a simple white-space character, enabling you to use multiple lines to write your commands.  File: gnuastro.info, Node: Acknowledgments, Prev: Conventions, Up: Introduction 1.11 Acknowledgments ==================== The list of Gnuastro authors is available at the start of this book and the ‘AUTHORS’ file in the source code. Here the authors wish to gratefully acknowledge the help and support they received from other people and institutions who had an indirect (not committed in the version controlled history) role in Gnuastro. The plain text file ‘THANKS’ which is distributed along with the source code also contains this list. The Japanese Ministry of Science and Technology (MEXT) scholarship for Mohammad Akhlaghi’s Masters and PhD period in Tohoku University Astronomical Institute had an instrumental role in the long term learning and planning that made the idea of Gnuastro possible. The very critical view points of Professor Takashi Ichikawa (Mohammad’s adviser) were also instrumental in the initial ideas and creation of Gnuastro. The European Research Council (ERC) advanced grant 339659-MUSICOS (Principal investigator: Roland Bacon) was vital in the growth and expansion of Gnuastro, enabling a thorough re-write of the core functionality of all libraries and programs, turning Gnuastro into the large collection of generic programs and libraries it is today. In general, we would like to gratefully thank the following people for their useful and constructive comments and suggestions (in alphabetical order by family name): Marjan Akbari, Roland Bacon, Karl Berry, Leindert Boogaard, Nicolas Bouché, Fernando Buitrago, Adrian Bunk, Rosa Calvi, Benjamin Clement, Antonio Diaz Diaz, Thérèse Godefroy, Madusha Gunawardhana, Stephen Hamer, Takashi Ichikawa, Raúl Infante Sainz, Brandon Invergo, Aurélien Jarno, Lee Kelvin, Mohammad-Reza Khellat, Floriane Leclercq, Alan Lefor, Guillaume Mahler, Francesco Montanari, William Pence, Bob Proulx, Yahya Sefidbakht, Alejandro Serrano Borlaff, Lee Spitler, Richard Stallman, Ole Streicher, Alfred M. Szmidt, Ignacio Trujillo, David Valls-Gabaud and Christopher Willmer. The GNU French Translation Team is also managing the French version of the top Gnuastro webpage which we highly appreciate. Finally we should thank all the (sometimes anonymous) people in various online forums which patiently answered all our small (but important) technical questions. All work on Gnuastro has been voluntary, but the authors are most grateful to the following institutions (in chronological order) for hosting us in our research: Ministry of education, culture, sports, science and technology (MEXT), Japan. Tohoku University Astronomical Institute, Sendai, Japan. University of Salento, Lecce, Italy. Centre national de la recherche scientifique (CNRS), France. Centre de Recherche Astrophysique de Lyon, University of Lyon 1, France.  File: gnuastro.info, Node: Tutorials, Next: Installation, Prev: Introduction, Up: Top 2 Tutorials *********** In this chapter we give several tutorials or cookbooks on how to use the various tools in Gnuastro for your scientific purposes. In these tutorials, we have intentionally avoided too many cross references to make it more easily readable. To get more information about a particular program, you can visit the section with the same name as the program in this book. Each program section starts by explaining the general concepts behind what it does. If you only want to see an explanation of the options and arguments of any program, see the subsection titled ‘Invoking ProgramName’. See *note Conventions::, for an explanation of the conventions we use in the example codes through the book. The tutorials in this section use a fictional setting of some historical figures in the history of astronomy. We have tried to show how Gnuastro would have been helpful for them in making their discoveries if there were GNU/Linux computers in their times! Please excuse us for any historical inaccuracy, this is not intended to be a historical reference. This form of presentation can make the tutorials more pleasant and entertaining to read while also being more practical (explaining from a user’s point of view)(1). The main reference for the historical facts mentioned in these fictional settings was Wikipedia. * Menu: * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. * General program usage tutorial:: Usage of all programs in a good way. ---------- Footnotes ---------- (1) This form of presenting a tutorial was influenced by the PGF/TikZ and Beamer manuals. The first provides graphic capabilities, while with the second you can make presentation slides in TeX and LaTeX. In these manuals, Till Tantau (author of the manual) uses Euclid as the protagonist. There are also some nice words of wisdom for Unix-like systems called “Rootless Rootâ€: . These also have a similar style but they use a mythical figure named Master Foo. If you already have some experience in Unix-like systems, you will definitely find these “Unix Koans†very entertaining.  File: gnuastro.info, Node: Hubble visually checks and classifies his catalog, Next: Sufi simulates a detection, Prev: Tutorials, Up: Tutorials 2.1 Hubble visually checks and classifies his catalog ===================================================== In 1924 Hubble(1) announced his discovery that some of the known nebulous objects are too distant to be within the the Milky Way (or Galaxy) and that they were probably distant Galaxies(2) in their own right. He had also used them to show that the redshift of the nebulae increases with their distance. So now he wants to study them more accurately to see what they actually are. Since they are nebulous or amorphous, they can’t be modeled (like stars that are always a point) easily. So there is no better way to distinguish them than to visually inspect them and see if it is possible to classify these nebulae or not. Hubble has stored all the FITS images of the objects he wants to visually inspect in his ‘/mnt/data/images’ directory. He has also stored his catalog of extra-galactic nebulae in ‘/mnt/data/catalogs/extragalactic.txt’. Any normal user on his GNU/Linux system (including himself) only has read access to the contents of the ‘/mnt/data’ directory. He has done this by running this command as root: # chmod -R 755 /mnt/data Hubble has done this intentionally to avoid mistakenly deleting or modifying the valuable images he has taken at Mount Wilson while he is working as an ordinary user. Retaking all those images and data is simply not an option. In fact they are also in another hard disk (‘/dev/sdb1’). So if the hard disk which stores his GNU/Linux distribution suddenly malfunctions due to work load, his data is not in harms way. That hard disk is only mounted to this directory when he wants to use it with the command: # mount /dev/sdb1 /mnt/data In short, Hubble wants to keep his data safe and fortunately by default Gnuastro allows for this. Hubble creates a temporary ‘visualcheck’ directory in his home directory for this check. He runs the following commands to make the directory and change to it(3): $ mkdir ~/visualcheck $ cd ~/visualcheck $ pwd /home/edwin/visualcheck $ ls Hubble has multiple images in ‘/mnt/data/images’, some of his targets might be on the edges of an image and so several images need to be stitched to give a good view of them. Also his extra-galactic targets belong to various pointings in the sky, so they are not in one large image. Gnuastro’s Crop is just the program he wants. The catalog in ‘extragalactic.txt’ is a plain text file which stores the basic information of all his known 200 extra-galactic nebulae. In its second column it has each object’s Right Ascension (the first column is a label he has given to each object) and in the third the object’s declination. $ astcrop --coordcol=2 --coordcol=3 /mnt/data/images/*.fits \ --mode=wcs /mnt/data/catalogs/extragalactic.txt Crop started on Tue Jun 14 10:18:11 1932 ---- ./4_crop.fits 1 1 ---- ./2_crop.fits 1 1 ---- ./1_crop.fits 1 1 [[[ Truncated middle of list ]]] ---- ./198_crop.fits 1 1 ---- ./195_crop.fits 1 1 - 200 images created. - 200 were filled in the center. - 0 used more than one input. Crop finished in: 2.429401 (seconds) Hubble already knows that thread allocation to the the CPU cores is asynchronous. Hence each time you run it, the order of which job gets done first differs. When using Crop the order of outputs is irrelevant since each crop is independent of the rest. This is why the crops are not necessarily created in the same input order. He is satisfied with the default width of the outputs (which he inspected by running ‘$ astcrop -P’). If he wanted a different width for the cropped images, he could do that with the ‘--wwidth’ option which accepts a value in arc-seconds. When he lists the contents of the directory again he finds his 200 objects as separate FITS images. $ ls 1_crop.fits 2_crop.fits ... 200_crop.fits The FITS image format was not designed for efficient/fast viewing, but mainly for accurate storing of the data. So he chooses to convert the cropped images to a more common image format to view them more quickly and easily through standard image viewers (which load much faster than FITS image viewer). JPEG is one of the most recognized image formats that is supported by most image viewers. Fortunately Gnuastro has just such a tool to convert various types of file types to and from each other: ConvertType. Hubble has already heard of GNU Parallel from one of his colleagues at Mount Wilson Observatory. It allows multiple instances of a command to be run simultaneously on the system, so he uses it in conjunction with ConvertType to convert all the images to JPEG. $ parallel astconvertt -ojpg ::: *_crop.fits For his graphical user interface Hubble is using GNOME which is the default in most distributions in GNU/Linux. The basic image viewer in GNOME is the Eye of GNOME, which has the executable file name ‘eog’ (4). Since he has used it before, he knows that once it opens an image, he can use the or keys on the keyboard to go to the next image in the directory or the key to go the previous image. So he opens the image of the first object with the command below and with his cup of coffee in his other hand, he flips through his targets very fast to get a good initial impression of the morphologies of these extra-galactic nebulae. $ eog 1_crop.jpg Hubble’s cup of coffee is now finished and he also got a nice general impression of the shapes of the nebulae. He tentatively/mentally classified the objects into three classes while doing the visual inspection. One group of the nebulae have a very simple elliptical shape and seem to have no internal special structure, so he gives them code 1. Another clearly different class are those which have spiral arms which he associates with code 2 and finally there seems to be a class of nebulae in between which appear to have a disk but no spiral arms, he gives them code 3. Now he wants to know how many of the nebulae in his extra-galactic sample are within each class. Repeating the same process above and writing the results on paper is very time consuming and prone to errors. Fortunately Hubble knows the basics of GNU Bash shell programming, so he writes the following short script with a loop to help him with the job. After all, computers are made for us to operate and knowing basic shell programming gives Hubble this ability to creatively operate the computer as he wants. So using GNU Emacs(5) (his favorite text editor) he puts the following text in a file named ‘classify.sh’. for name in *.jpg do eog $name & processid=$! echo -n "$name belongs to class: " read class echo $name $class >> classified.txt kill $processid done Fortunately GNU Emacs or even simpler editors like Gedit (part of the GNOME graphical user interface) will display the variables and shell constructs in different colors which can really help in understanding the script. Put simply, the ‘for’ loop gets the name of each JPEG file in the directory this script is run in and puts it in ‘name’. In the shell, the value of a variable is used by putting a ‘$’ sign before the variable name. Then Eye of GNOME is run on the image in the background to show him that image and its process ID is saved internally (this is necessary to close Eye of GNOME later). The shell then prompts the user to specify a class and after saving it in ‘class’, it prints the file name and the given class in the next line of a file named ‘classified.txt’. To make the script executable (so he can run it later any time he wants) he runs: $ chmod +x classify.sh Now he is ready to do the classification, so he runs the script: $ ./classify.sh In the end he can delete all the JPEG and FITS files along with Crop’s log file with the following short command. The only files remaining are the script and the result of the classification. $ rm *.jpg *.fits astcrop.txt $ ls classified.txt classify.sh He can now use ‘classified.txt’ as input to a plotting program to plot the histogram of the classes and start making interpretations about what these nebulous objects that are outside of the Galaxy are. ---------- Footnotes ---------- (1) Edwin Powell Hubble (1889 – 1953 A.D.) was an American astronomer who can be considered as the father of extra-galactic astronomy, by proving that some nebulae are too distant to be within the Galaxy. He then went on to show that the universe appears to expand and also done a visual classification of the galaxies that is known as the Hubble fork. (2) Note that at that time, “Galaxy†was a proper noun used to refer to the Milky way. The concept of a galaxy as we define it today had not yet become common. Hubble played a major role in creating today’s concept of a galaxy. (3) The ‘pwd’ command is short for “Print Working Directory†and ‘ls’ is short for “list†which shows the contents of a directory. (4) Eye of GNOME is only available for users of the GNOME graphical desktop environment which is the default in most GNU/Linux distributions. If you use another graphical desktop environment, replace ‘eog’ with any other image viewer. (5) This can be done with any text editor  File: gnuastro.info, Node: Sufi simulates a detection, Next: General program usage tutorial, Prev: Hubble visually checks and classifies his catalog, Up: Tutorials 2.2 Sufi simulates a detection ============================== It is the year 953 A.D. and Sufi(1) is in Shiraz as a guest astronomer. He had come there to use the advanced 123 centimeter astrolabe for his studies on the Ecliptic. However, something was bothering him for a long time. While mapping the constellations, there were several non-stellar objects that he had detected in the sky, one of them was in the Andromeda constellation. During a trip he had to Yemen, Sufi had seen another such object in the southern skies looking over the Indian ocean. He wasn’t sure if such cloud-like non-stellar objects (which he was the first to call ‘SahÄbi’ in Arabic or ‘nebulous’) were real astronomical objects or if they were only the result of some bias in his observations. Could such diffuse objects actually be detected at all with his detection technique? He still had a few hours left until nightfall (when he would continue his studies on the ecliptic) so he decided to find an answer to this question. He had thoroughly studied Claudius Ptolemy’s (90 – 168 A.D) Almagest and had made lots of corrections to it, in particular in measuring the brightness. Using his same experience, he was able to measure a magnitude for the objects and wanted to simulate his observation to see if a simulated object with the same brightness and size could be detected in a simulated noise with the same detection technique. The general outline of the steps he wants to take are: 1. Make some mock profiles in an oversampled image. The initial mock image has to be oversampled prior to convolution or other forms of transformation in the image. Through his experiences, Sufi knew that this is because the image of heavenly bodies is actually transformed by the atmosphere or other sources outside the atmosphere (for example gravitational lenses) prior to being sampled on an image. Since that transformation occurs on a continuous grid, to best approximate it, he should do all the work on a finer pixel grid. In the end he can re-sample the result to the initially desired grid size. 2. Convolve the image with a PSF image that is oversampled to the same value as the mock image. Since he wants to finish in a reasonable time and the PSF kernel will be very large due to oversampling, he has to use frequency domain convolution which has the side effect of dimming the edges of the image. So in the first step above he also has to build the image to be larger by at least half the width of the PSF convolution kernel on each edge. 3. With all the transformations complete, the image should be re-sampled to the same size of the pixels in his detector. 4. He should remove those extra pixels on all edges to remove frequency domain convolution artifacts in the final product. 5. He should add noise to the (until now, noise-less) mock image. After all, all observations have noise associated with them. Fortunately Sufi had heard of GNU Astronomy Utilities from a colleague in Isfahan (where he worked) and had installed it on his computer a year before. It had tools to do all the steps above. He had used MakeProfiles before, but wasn’t sure which columns he had chosen in his user or system wide configuration files for which parameters, see *note Configuration files::. So to start his simulation, Sufi runs MakeProfiles with the ‘-P’ option to make sure what columns in a catalog MakeProfiles currently recognizes and the output image parameters. In particular, Sufi is interested in the recognized columns (shown below). $ astmkprof -P [[[ ... Truncated lines ... ]]] # Output: type float32 # Type of output: e.g., int16, float32, etc... naxis 1000,1000 # Number of pixels along first FITS axis. oversample 5 # Scale of oversampling (>0 and odd). [[[ ... Truncated lines ... ]]] # Columns, by info (see `--searchin'), or number (starting from 1): ccol 2 # Center along first FITS axis (horizontal). ccol 3 # Center along second FITS axis (vertical). fcol 4 # sersic (1), moffat (2), gaussian (3), # point (4), flat (5), circumference (6). rcol 5 # Effective radius or FWHM in pixels. ncol 6 # Sersic index or Moffat beta. pcol 7 # Position angle. qcol 8 # Axis ratio. mcol 9 # Magnitude. tcol 10 # Truncation in units of radius or pixels. [[[ ... Truncated lines ... ]]] In Gnuastro, column counting starts from 1, so the columns are ordered such that the first column (number 1) can be an ID he specifies for each object (and MakeProfiles ignores), each subsequent column is used used for another property of the profile. It is also possible to use column names for the values of these options and change these defaults, but Sufi preferred to stick to the defaults. Fortunately MakeProfiles has the capability to also make the PSF which is to be used on the mock image and using the ‘--prepforconv’ option, he can also make the mock image to be larger by the correct amount and all the sources to be shifted by the correct amount. For his initial check he decides to simulate the nebula in the Andromeda constellation. The night he was observing, the PSF had roughly a FWHM of about 5 pixels, so as the first row (profile), he defines the PSF parameters and sets the radius column (‘rcol’ above, fifth column) to ‘5.000’, he also chooses a Moffat function for its functional form. Remembering how diffuse the nebula in the Andromeda constellation was, he decides to simulate it with a mock Sérsic index 1.0 profile. He wants the output to be 500 pixels by 500 pixels, so he puts the mock profile in the center. Looking at his drawings of it, he decides a reasonable effective radius for it would be 40 pixels on this image pixel scale, he sets the axis ratio and position angle to approximately correct values too and finally he sets the total magnitude of the profile to 3.44 which he had accurately measured. Sufi also decides to truncate both the mock profile and PSF at 5 times the respective radius parameters. In the end he decides to put four stars on the four corners of the image at very low magnitudes as a visual scale. Using all the information above, he creates the catalog of mock profiles he wants in a file named ‘cat.txt’ (short for catalog) using his favorite text editor and stores it in a directory named ‘simulationtest’ in his home directory. [The ‘cat’ command prints the contents of a file, short for concatenation. So please copy-paste the lines after “‘cat cat.txt’†into ‘cat.txt’ when the editor opens in the steps above it, note that there are 7 lines, first one starting with <#>]: $ mkdir ~/simulationtest $ cd ~/simulationtest $ pwd /home/rahman/simulationtest $ emacs cat.txt $ ls cat.txt $ cat cat.txt # Column 4: PROFILE_NAME [,str7] Radial profile's functional name 1 0.0000 0.0000 moffat 5.000 4.765 0.0000 1.000 30.000 5.000 2 250.00 250.00 sersic 40.00 1.000 -25.00 0.400 3.4400 5.000 3 50.000 50.000 point 0.000 0.000 0.0000 0.000 9.0000 0.000 4 450.00 50.000 point 0.000 0.000 0.0000 0.000 9.2500 0.000 5 50.000 450.00 point 0.000 0.000 0.0000 0.000 9.5000 0.000 6 450.00 450.00 point 0.000 0.000 0.0000 0.000 9.7500 0.000 The zero-point magnitude for his observation was 18. Now he has all the necessary parameters and runs MakeProfiles with the following command: $ astmkprof --prepforconv --naxis=500,500 --zeropoint=18.0 cat.txt MakeProfiles started on Sat Oct 6 16:26:56 953 - 6 profiles read from cat.txt - Random number generator (RNG) type: mt19937 - Using 8 threads. ---- row 2 complete, 5 left to go ---- row 3 complete, 4 left to go ---- row 4 complete, 3 left to go ---- row 5 complete, 2 left to go ---- ./0_cat.fits created. ---- row 0 complete, 1 left to go ---- row 1 complete, 0 left to go - ./cat.fits created. 0.041651 seconds MakeProfiles finished in 0.267234 seconds $ls 0_cat.fits cat.fits cat.txt The file ‘0_cat.fits’ is the PSF Sufi had asked for and ‘cat.fits’ is the image containing the other 5 objects. The PSF is now available to him as a separate file for the convolution step. While he was preparing the catalog, one of his students approached him and was also following the steps. When he opened the image, the student was surprised to see that all the stars are only one pixel and not in the shape of the PSF as we see when we image the sky at night. So Sufi explained to him that the stars will take the shape of the PSF after convolution and this is how they would look if we didn’t have an atmosphere or an aperture when we took the image. The size of the image was also surprising for the student, instead of 500 by 500, it was 2630 by 2630 pixels. So Sufi had to explain why oversampling is very important for parts of the image where the flux change is significant over a pixel. Sufi then explained to him that after convolving we will re-sample the image to get our originally desired size. To convolve the image, Sufi ran the following command: $ astconvolve --kernel=0_cat.fits cat.fits Convolve started on Mon Apr 6 16:35:32 953 - Using 8 CPU threads. - Input: cat.fits (hdu: 1) - Kernel: 0_cat.fits (hdu: 1) - Input and Kernel images padded. 0.075541 seconds - Images converted to frequency domain. 6.728407 seconds - Multiplied in the frequency domain. 0.040659 seconds - Converted back to the spatial domain. 3.465344 seconds - Padded parts removed. 0.016767 seconds Convolve finished in: 10.422161 seconds $ls 0_cat.fits cat_convolved.fits cat.fits cat.txt When convolution finished, Sufi opened the ‘cat_convolved.fits’ file and showed the effect of convolution to his student and explained to him how a PSF with a larger FWHM would make the points even wider. With the convolved image ready, they were prepared to re-sample it to the original pixel scale Sufi had planned [from the ‘$ astmkprof -P’ command above, recall that MakeProfiles had oversampled the image by 5 times]. Sufi explained the basic concepts of warping the image to his student and ran Warp with the following command: $ astwarp --scale=1/5 --centeroncorner cat_convolved.fits Warp started on Mon Apr 6 16:51:59 953 Using 8 CPU threads. Input: cat_convolved.fits (hdu: 1) matrix: 0.2000 0.0000 0.4000 0.0000 0.2000 0.4000 0.0000 0.0000 1.0000 $ ls 0_cat.fits cat_convolved_scaled.fits cat.txt cat_convolved.fits cat.fits $ astfits -p cat_convolved_scaled.fits | grep NAXIS NAXIS = 2 / number of data axes NAXIS1 = 526 / length of data axis 1 NAXIS2 = 526 / length of data axis 2 ‘cat_convolved_warped.fits’ now has the correct pixel scale. However, the image is still larger than what we had wanted, it is 526 ($500+13+13$) by 526 pixels. The student is slightly confused, so Sufi also resamples the PSF with the same scale and shows him that it is 27 ($2\times13+1$) by 27 pixels. Sufi goes on to explain how frequency space convolution will dim the edges and that is why he added the ‘--prepforconv’ option to MakeProfiles, see *note If convolving afterwards::. Now that convolution is done, Sufi can remove those extra pixels using Crop with the command below. Crop’s ‘--section’ option accepts coordinates inclusively and counting from 1 (according to the FITS standard), so the crop’s first pixel has to be 14, not 13. $ astcrop cat_convolved_scaled.fits --section=14:*-13,14:*-13 \ --zeroisnotblank Crop started on Sat Oct 6 17:03:24 953 - Read metadata of 1 image. 0.001304 seconds ---- ...nvolved_scaled_cropped.fits created: 1 input. Crop finished in: 0.027204 seconds $ls 0_cat.fits cat_convolved_scaled_cropped.fits cat.fits cat_convolved.fits cat_convolved_scaled.fits cat.txt Finally, ‘cat_convolved_scaled_cropped.fits’ has the same dimensions as Sufi had desired in the beginning. All this trouble was certainly worth it because now there is no dimming on the edges of the image and the profile centers are more accurately sampled. The final step to simulate a real observation would be to add noise to the image. Sufi set the zeropoint magnitude to the same value that he set when making the mock profiles and looking again at his observation log, he had measured the background flux near the nebula had a magnitude of 7 that night. So using these values he ran MakeNoise: $ astmknoise --zeropoint=18 --background=7 --output=out.fits \ cat_convolved_warped_crop.fits MakeNoise started on Mon Apr 6 17:05:06 953 - Generator type: mt19937 - Generator seed: 1428318100 MakeNoise finished in: 0.033491 (seconds) $ls 0_cat.fits cat_convolved_scaled_cropped.fits cat.fits out.fits cat_convolved.fits cat_convolved_scaled.fits cat.txt The ‘out.fits’ file now contains the noised image of the mock catalog Sufi had asked for. Seeing how the ‘--output’ option allows the user to specify the name of the output file, the student was confused and wanted to know why Sufi hadn’t used it before? Sufi then explained to him that for intermediate steps it is best to rely on the automatic output, see *note Automatic output::. Doing so will give all the intermediate files the same basic name structure, so in the end you can simply remove them all with the Shell’s capabilities. So Sufi decided to show this to the student by making a shell script from the commands he had used before. The command-line shell has the capability to read all the separate input commands from a file. This is very useful when you want to do the same thing multiple times, with only the names of the files or minor parameters changing between the different instances. Using the shell’s history (by pressing the up keyboard key) Sufi reviewed all the commands and then he retrieved the last 5 commands with the ‘$ history 5’ command. He selected all those lines he had input and put them in a text file named ‘mymock.sh’. Then he defined the ‘edge’ and ‘base’ shell variables for easier customization later. Finally, before every command, he added some comments (lines starting with <#>) for future readability. # Basic settings: edge=13 base=cat # Remove any existing image to avoid confusion. rm out.fits # Run MakeProfiles to create an oversampled FITS image. astmkprof --prepforconv --naxis=500,500 --zeropoint=18.0 "$base".txt # Convolve the created image with the kernel. astconvolve --kernel=0_"$base".fits "$base".fits # Scale the image back to the intended resolution. astwarp --scale=1/5 --centeroncorner "$base"_convolved.fits # Crop the edges out (dimmed during convolution). `--section' accepts # inclusive coordinates, so the start of start of the section must be # one pixel larger than its end. st_edge=$(( edge + 1 )) astcrop "$base"_convolved_scaled.fits --zeroisnotblank \ --section=$st_edge:*-$edge,$st_edge:*-$edge # Add noise to the image. astmknoise --zeropoint=18 --background=7 --output=out.fits \ "$base"_convolved_scaled_cropped.fits # Remove all the temporary files. rm 0*.fits cat*.fits He used this chance to remind the student of the importance of comments in code or shell scripts: when writing the code, you have a very good mental picture of what you are doing, so writing comments might seem superfluous and excessive. However, in one month when you want to re-use the script, you have lost that mental picture and rebuilding it is can be very time-consuming and frustrating. The importance of comments is further amplified when you want to share the script with a friend/colleague. So it is very good to accompany any script/code with useful comments while you are writing it (have a good mental picture of what/why you are doing something). Sufi then explained to the eager student that you define a variable by giving it a name, followed by an ‘=’ sign and the value you want. Then you can reference that variable from anywhere in the script by calling its name with a ‘$’ prefix. So in the script whenever you see ‘$base’, the value we defined for it above is used. If you use advanced editors like GNU Emacs or even simpler ones like Gedit (part of the GNOME graphical user interface) the variables will become a different color which can really help in understanding the script. We have put all the ‘$base’ variables in double quotation marks (‘"’) so the variable name and the following text do not get mixed, the shell is going to ignore the ‘"’ after replacing the variable value. To make the script executable, Sufi ran the following command: $ chmod +x mymock.sh Then finally, Sufi ran the script, simply by calling its file name: $ ./mymock.sh After the script finished, the only file remaining is the ‘out.fits’ file that Sufi had wanted in the beginning. Sufi then explained to the student how he could run this script anywhere that he has a catalog if the script is in the same directory. The only thing the student had to modify in the script was the name of the catalog (the value of the ‘base’ variable in the start of the script) and the value to the ‘edge’ variable if he changed the PSF size. The student was also very happy to hear that he won’t need to make it executable again when he makes changes later, it will remain executable unless he explicitly changes the executable flag with ‘chmod’. The student was really excited, since now, through simple shell scripting, he could really speed up his work and run any command in any fashion he likes allowing him to be much more creative in his works. Until now he was using the graphical user interface which doesn’t have such a facility and doing repetitive things on it was really frustrating and some times he would make mistakes. So he left to go and try scripting on his own computer. Sufi could now get back to his own work and see if the simulated nebula which resembled the one in the Andromeda constellation could be detected or not. Although it was extremely faint(2), fortunately it passed his detection tests and he wrote it in the draft manuscript that would later become “Book of fixed starsâ€. He still had to check the other nebula he saw from Yemen and several other such objects, but they could wait until tomorrow (thanks to the shell script, he only has to define a new catalog). It was nearly sunset and they had to begin preparing for the night’s measurements on the ecliptic. ---------- Footnotes ---------- (1) Abd al-rahman Sufi (903 – 986 A.D.), also known in Latin as Azophi was an Iranian astronomer. His manuscript “Book of fixed stars†contains the first recorded observations of the Andromeda galaxy, the Large Magellanic Cloud and seven other non-stellar or ‘nebulous’ objects. (2) The brightness of a diffuse object is added over all its pixels to give its final magnitude, see *note Flux Brightness and magnitude::. So although the magnitude 3.44 (of the mock nebula) is orders of magnitude brighter than 6 (of the stars), the central galaxy is much fainter. Put another way, the brightness is distributed over a large area in the case of a nebula.  File: gnuastro.info, Node: General program usage tutorial, Prev: Sufi simulates a detection, Up: Tutorials 2.3 General program usage tutorial ================================== Measuring colors of astronomical objects in broad-band or narrow-band images is one of the most basic and common steps in astronomical analysis. Here, we will use Gnuastro’s programs to detect objects in a Hubble Space Telescope (HST) image and measure their colors. We will use the eXtreme Deep Field (https://archive.stsci.edu/prepds/xdf) dataset. Like almost all astronomical surveys, this dataset is free for download and usable by the public. This tutorial was first prepared for the “Exploring the Ultra-Low Surface Brightness Universe†workshop (November 2017) at the International Space Science Institute (ISSI) in Bern, Switzerland. We would like to thank them and the attendees for a very fruitful week. You will need the following tools in this tutorial: Gnuastro, SAO DS9 (1), GNU Wget(2), and AWK (most common implementation is GNU AWK(3)). *Type the example commands:* Try to type the example commands on your terminal and don’t simply copy and paste them. This will help simulate future situations when you are processing your own datasets. A handy feature of Gnuastro is that all program names start with ‘ast’. This will allow your command-line processor to easily list and auto-complete Gnuastro’s programs for you. Try typing the following command (press key when you see ‘’) to see the list: $ ast Any program that starts with ‘ast’ (including all Gnuastro programs) will be shown. By choosing the subsequent characters of your desired program and pressing <> again, the list will narrow down and the program name will auto-complete once your input characters are unambiguous. In short, you often don’t need to type the full name of the program you want to run. Gnuastro contains a large number of programs and it is natural to forget the details of each program’s options. Therefore, before starting the analysis, let’s review how you can refresh your memory any time you want on the command-line while working (without taking your hands off the keyboard). This book comes with your installation, so it will always correspond to your installed version of Gnuastro. Please see *note Info:: for more. GNU Info(4) is the program in charge of displaying the manual on the command-line. To see this whole book on your command-line, please run the following command and subsequent keys. Info has its own mini-environment, therefore we’ll show the keys that must be pressed in the mini-environment after a ‘->’ sign. You can also ignore anything after the ‘#’ sign in the middle of the line, they are only for your information. $ info gnuastro # Open the top of the manual. -> # All the book chapters. -> # Continue down: show sections. -> ... # Keep pressing space to go down. -> q # Quit Info, return to the command-line. The thing that greatly simplifies navigation in Info is the links (regions with an underline). You can immediately go to the next link in the page with the <> key and press <> on it to go into that part of the manual. Try the commands above again, but this time also use <> to go to the links and press <> on them to go to the respective section of the book. Then follow a few more links and go deeper into the book. To return to the previous page, press (small L). If you are searching for a specific phrase in the whole book (for example an option name), press and type your search phrase and end it with an <>. You don’t need to start from the top of the manual every time. For example, to get to *note Invoking astnoisechisel::, run the following command. In general, all programs have such an “Invoking ProgramName†section in this book. These sections are specifically for the description of inputs, outputs and configuration options of each program. You can access them directly for each program by giving its executable name to Info. $ info astnoisechisel The other sections don’t have such shortcuts. To directly access them from the command-line, you need to tell Info to look into Gnuastro’s manual, then look for the specific section (an unambiguous title is necessary). For example, if you only want to review/remember NoiseChisel’s *note Detection options:: or *note Segmentation options::), just run any of these commands. Note how case is irrelevant for Info when calling a title in this manner. $ info gnuastro "Detection options" $ info gnuastro "segmentation options" In general, Info is a wonderful and powerful way to access this whole book with detailed information about the programs you are running very fast. If you are not already familiar with it, please run the following command and just read along and do what it says to learn it. Don’t stop until you feel have become sufficiently fluent in it. Please invest the half an hour’s time necessary to start using Info comfortably. It will greatly improve your productivity and you will start reaping the rewards of this investment very soon. $ info info As a good scientist you need to feel comfortable to play with the features/options and avoid (be critical to) using default values as much as possible. On the other hand, our human memory is very limited, so it is important to be able to easily access any part of this book fast and remember the option names, what they do and their acceptable values. If you just want the option names and a short description, calling the program with the ‘--help’ option might also be a good solution like the first example below. If you know a few characters of the option name, you can feed the output to ‘grep’ like the second or third example commands. $ astnoisechisel --help $ astnoisechisel --help | grep quant $ astnoisechisel --help | grep check Let’s start the processing. First, to keep things clean, let’s create a ‘gnuastro-tutorial’ directory and continue all future steps in it: $ mkdir gnuastro-tutorial $ cd gnuastro-tutorial We will be using the near infra-red Wide Field Camera (http://www.stsci.edu/hst/wfc3) dataset. If you already have them in another directory (for example ‘XDFDIR’), you can set the ‘download’ directory to be a symbolic link to ‘XDFDIR’ with a command like this: ln -s XDFDIR download If the following images aren’t already present on your system, you can make a ‘download’ directory and download them there. $ mkdir download $ cd download $ xdfurl=http://archive.stsci.edu/pub/hlsp/xdf $ wget $xdfurl/hlsp_xdf_hst_wfc3ir-60mas_hudf_f105w_v1_sci.fits $ wget $xdfurl/hlsp_xdf_hst_wfc3ir-60mas_hudf_f160w_v1_sci.fits $ cd .. In this tutorial, we’ll just use these two filters. Later, you will probably need to download more filters, you can use the shell’s ‘for’ loop to download them all in series (one after the other(5)) with one command like the one below for the WFC3 filters. Put this command instead of the two ‘wget’ commands above. Recall that all the extra spaces, back-slashes (‘\’), and new lines can be ignored if you are typing on the lines on the terminal. $ for f in f105w f125w f140w f160w; do \ wget $xdfurl/hlsp_xdf_hst_wfc3ir-60mas_hudf_"$f"_v1_sci.fits; \ done First, let’s visually inspect the dataset. Let’s take F160W image as an example. Do the steps below with the other image(s) too (and later with any dataset that you want to work on). It is very important to understand your dataset visually. Note how ds9 doesn’t follow the GNU style of options where “long†and “short†options are preceded by ‘--’ and ‘-’ respectively (for example ‘--width’ and ‘-w’, see *note Options::). Ds9’s ‘-zscale’ option is a good scaling to highlight the low surface brightness regions, and as the name suggests, ‘-zoom to fit’ will fit the whole dataset in the window. If the window is too small, expand it with your mouse, then press the “zoom†button on the top row of buttons above the image, then in the row below it, press “zoom fitâ€. You can also zoom in and out by scrolling your mouse or the respective operation on your touch-pad when your cursor/pointer is over the image. $ ds9 download/hlsp_xdf_hst_wfc3ir-60mas_hudf_f160w_v1_sci.fits \ -zscale -zoom to fit The first thing you might notice is that the regions with no data have a value of zero in this image. The next thing might be that the dataset actually has two “depthâ€s (see *note Quantifying measurement limits::). The exposure time of the inner region is more than 4 times more than the outer parts. Fortunately the XDF survey webpage (above) contains the vertices of the deep flat WFC3-IR field. You can use those vertices in *note Crop:: to cutout this deep infra-red region from the larger image. We’ll make a directory called ‘flat-ir’ and keep the flat infra-red regions in that directory (with a ‘‘xdf-’’ suffix for a shorter and easier filename). $ mkdir flat-ir $ astcrop --mode=wcs -h0 --output=flat-ir/xdf-f105w.fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" \ download/hlsp_xdf_hst_wfc3ir-60mas_hudf_f105w_v1_sci.fits $ astcrop --mode=wcs -h0 --output=flat-ir/xdf-f160w.fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" \ download/hlsp_xdf_hst_wfc3ir-60mas_hudf_f160w_v1_sci.fits The only thing varying in the two calls to Gnuastro’s Crop program is the filter name. Therefore, to simplify the command, and later allow work on more filters, we can use the shell’s ‘for’ loop. Notice how the two places where the filter names (‘f105w’ and ‘f160w’) are used above have been replaced with ‘$f’ (the shell variable that ‘for’ is in charge of setting) below. To generalize this for more filters later, you can simply add the other filter names in the first line before the semi-colon (‘;’). $ for f in f105w f160w; do \ astcrop --mode=wcs -h0 --output=flat-ir/xdf-$f.fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" \ download/hlsp_xdf_hst_wfc3ir-60mas_hudf_"$f"_v1_sci.fits; \ done Please open these images and inspect them with the same ds9 commands you used above. You will see how it is completely flat now and doesn’t have varying depths. Another important result of this crop is that regions with no data now have a NaN (blank) value, not zero. Zero is a meaningful value and especially when using NoiseChisel, the input should have NaN values for pixels with no data, not zero. This is the deepest image we currently have of the sky. The first thing that comes to mind may be this: “How large is this field?â€. Let’s find the answer to this question with the commands below. The lines starting with ‘##’ are just comments for you to help in following the steps. Don’t type them on the terminal. The commands are intentionally repetitive in some places to better understand each step and also to demonstrate the beauty of command-line features like variables, pipes and loops. Later, if you would like to repeat this process on another dataset, you can just use commands 3, 7, and 9. *Use shell history:* Don’t forget to make effective use of your shell’s history. This is especially convenient when you just want to make a small change to your previous command. Press the “up†key on your keyboard (possibly multiple times) to see your previous command(s). ## (1) See the general statistics of non-blank pixel values. $ aststatistics flat-ir/xdf-f160w.fits ## (2) We only want the number of non-blank pixels. $ aststatistics flat-ir/xdf-f160w.fits --number ## (3) Keep the result of the command above in the shell variable `n'. $ n=$(aststatistics flat-ir/xdf-f160w.fits --number) ## (4) See what is stored the shell variable `n'. $ echo $n ## (5) Show all the FITS keywords of this image. $ astfits flat-ir/xdf-f160w.fits -h1 ## (6) The resolution (in degrees/pixel) is in the `CDELT' keywords. ## Only show lines that contain these characters, by feeding ## the output of the previous command to the `grep' program. $ astfits flat-ir/xdf-f160w.fits -h1 | grep CDELT ## (7) Save the resolution (same in both dimensions) in the variable ## `r'. The last part uses AWK to print the third `field' of its ## input line. The first two fields were `CDELT1' and `='. $ r=$(astfits flat-ir/xdf-f160w.fits -h1 | grep CDELT1 \ | awk '{print $3}') ## (8) Print the values of `n' and `r'. $ echo $n $r ## (9) Use the number of pixels (first number passed to AWK) and ## length of each pixel's edge (second number passed to AWK) ## to estimate the area of the field in arc-minutes squared. $ area=(echo $n $r | awk '{print $1 * ($2^2) * 3600}') The area of this field is 4.03817 (or 4.04) arc-minutes squared. Just for comparison, this is roughly 175 times smaller than the average moon’s angular area (with a diameter of 30arc-minutes or half a degree). *AWK for table/value processing:* AWK is a powerful and simple tool for text processing. Above (and further below) some simple examples are shown. GNU AWK (the most common implementation) comes with a free and wonderful book (https://www.gnu.org/software/gawk/manual/) in the same format as this book which will allow you to master it nicely. Just like this manual, you can also access GNU AWK’s manual on the command-line whenever necessary without taking your hands off the keyboard as described above. This takes us to the second question that you have probably asked yourself when you saw the field for the first time: “How large is this area at different redshifts?â€. To get a feeling of the tangential area that this field covers at redshift 2, you can use *note CosmicCalculator::. In particular, you need the tangential distance covered by 1 arc-second as raw output. Combined with the field’s area, we can then calculate the tangential distance in Mega Parsecs squared ($Mpc^2$). ## Print general cosmological properties at redshift 2. $ astcosmiccal -z2 ## When given a "Specific calculation" option, CosmicCalculator ## will just print that particular calculation. See the options ## under this title in the output of `--help' for more. $ astcosmiccal --help ## Only print the "Tangential dist. covered by 1arcsec at z (kpc)". ## in units of kpc/arc-seconds. $ astcosmiccal -z2 --arcsectandist ## Convert this distance to kpc^2/arcmin^2 and save in `k'. $ k=$(astcosmiccal -z2 --arcsectandist | awk '{print ($1*60)^2}') ## Multiply by the area of the field (in arcmin^2) and divide by ## 10^6 to return value in Mpc^2. $ echo $k $area | awk '{print $1 * $2 / 1e6}' At redshift 2, this field therefore covers 1.07145 $Mpc^2$. If you would like to see how this tangential area changes with redshift, you can use a shell loop like below. $ for z in 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0; do \ k=$(astcosmiccal -z$z --arcsectandist); \ echo $z $k $area | awk '{print $1, ($2*60)^2 * $3 / 1e6}'; \ done Fortunately, the shell has a very useful tool/program to print a sequence of numbers that is nicely called ‘seq’. You can use it instead of typing all the different redshifts in this example. For example the loop below will print the same range of redshifts (between 0.5 and 5) but with increments of 0.1. $ for z in $(seq 0.5 0.1 5); do \ k=$(astcosmiccal -z$z --arcsectandist); \ echo $z $k $area | awk '{print $1, ($2*60)^2 * $3 / 1e6}'; \ done If you want a fast result and commonly need such processing for a larger number of redshifts, the command above can be slow. This is because the CosmicCalculator program has a lot of overhead: it has to parse the command-line and all configuration files (see below). These are both human-readable characters, not computer-readable bits. CosmicCalculator then has to check the sanity of its inputs and check which of its many options you have asked for. It has to do all of these for every redshift. To greatly speed up the processing, Gnuastro gives you direct access to the root work-horse of CosmicCalculator without all that overhead: *note Gnuastro library::. Using Gnuastro’s library, you can write your own tiny little program for this same calculation, without all that extra overhead of CosmicCalculator (or any of Gnuastro’s programs, see *note Library::). For this particular job, you want Gnuastro’s *note Cosmology library::. Here is one example: put the following small C program in a file called ‘myprogram.c’. #include #include #include #include int main(void) { double area=4.03817; /* Area of field (arcmin^2). */ double z, adist, tandist; /* Temporary variables. */ /* Constants from Plank 2015 (Paper XIII, A&A 594, 2016) */ double H0=67.74, olambda=0.6911, omatter=0.3089, oradiation=0; /* Do the same thing for all redshifts (z) between 0.1 and 5. */ for(z=0.1; z<5; z+=0.1) { /* Calculate the angular diameter distance. */ adist=gal_cosmology_angular_distance(z, H0, olambda, omatter, oradiation); /* Calculate the tangential distance of one arcsecond. */ tandist = adist * 1000 * M_PI / 3600 / 180; /* Print the redshift and area. */ printf("%-5.2f %g\n", z, pow(tandist * 60,2) * area / 1e6); } /* Tell the system that everything finished successfully. */ return EXIT_SUCCESS; } To build and run this C program, you can use *note BuildProgram::. It is designed to manage Gnuastro’s dependencies, compile the program you give it and then run it. In short, it hides all the complexities of compiling, linking and running C programs based on Gnuastro’s library. The library will later be usable higher level languages like Python or Julia, for now it is only usable by C and C++ programs. $ astbuildprog myprogram.c See how much faster this is compared to the shell loop we wrote above? You might have noticed that a new file called ‘myprogram’ is also created in the directory. This is the compiled program that was created and run by the command above (its in binary machine code, not human-readable any more). You can run it again to get the same results with a command like this: $ ./myprogram The efficiency of ‘myprogram’ compared to CosmicCalculator is because the requested processing is faster/comparable to the overheads. For other programs that take large input datasets (images for example), the overhead is usually negligible compared to the processing. In such cases, the libraries are only useful if you want a different/new processing compared to the functionalities in Gnuastro’s existing programs. Gnuastro has a large library which all the programs use for various steps their processing. For the full list of available functions classified by context, please see *note Gnuastro library::. Gnuastro’s library and BuildProgram are created to make it easy for you to use these powerful features and get to your scientific results as efficiently (fast) and accurately as possible. Several other complete working examples (involving images and tables) of Gnuastro’s libraries can be see in *note Library demo programs::. We’ll stop with the libraries at this point in this tutorial and get back to Gnuastro’s already built programs which ready to be used on the command-line. None of Gnuastro’s programs keep a default value internally within their code. However, when you ran CosmicCalculator with the ‘-z2’ option above, it completed its processing and printed results. So where did the “default†cosmological parameter values (like the matter density and etc) come from? The values come from the command-line or a configuration file (see *note Configuration file precedence::). CosmicCalculator has a very limited set of parameters and doesn’t need any particular file inputs. Therefore, we’ll use it to discuss configuration files which are an important part of all Gnuastro’s programs (see *note Configuration files::). Once you get comfortable with configuration files, you can easily do the same for the options of all Gnuastro programs. For example, NoiseChisel has the largest number of options in the programs. Therefore configuration files will be very useful for it when you use different datasets (with different noise properties or in different research contexts). The configuration of each program (besides its version) is vital for the reproducibility of your results, so it is very important to manage them properly. As we saw above, the full list of the options in all Gnuastro programs can be seen with the ‘--help’ option. Try calling it with CosmicCalculator as shown below. Note how options are grouped by context to make it easier to find your desired option. However, in each group, options are ordered alphabetically. $ astcosmiccal --help The options that need a value have an <=> sign after their long version and ‘FLT’, ‘INT’ or ‘STR’ for floating point numbers, integer numbers and strings (filenames for example) respectively. All options have a long format and some have a short format (a single character), for more see *note Options::. When you are using a program, it is often necessary to check the value the option has just before the program starts its processing. In other words, after it has parsed the command-line options and all configuration files. You can see the values of all options that need one with the ‘--printparams’ or ‘-P’ option that is common to all programs (see *note Common options::). In the command below, try replacing ‘-P’ with ‘--printparams’ to see how both do the same operation. $ astcosmiccal -P Let’s say you want a different Hubble constant. Try running the following command to see how the Hubble constant in the output of the command above has changed. Afterwards, delete the ‘-P’ and add a ‘-z2’ to see the results with the new cosmology (or configuration). $ astcosmiccal -P --H0=70 From the output of the ‘--help’ option, note how the option for Hubble constant has both short (‘-H’) and long (‘--H0’) formats. One final note is that the equal (<=>) sign is not mandatory. In the short format, the value can stick to the actual option (the short option name is just one character after-all and thus easily identifiable) and in the long format, a white-space character is also enough. $ astcosmiccal -H70 -z2 $ astcosmiccal --H0 70 -z2 --arcsectandisk Let’s assume that in one project, you want to only use rounded cosmological parameters (H0 of 70km/s/Mpc and matter density of 0.3). You should therefore run CosmicCalculator like this: $ astcosmiccal --H0=70 --olambda=0.7 --omatter=0.3 -z2 But having to type these extra options every time you run CosmicCalculator will be prone to errors (typos in particular) and also will be frustrating and slow. Therefore in Gnuastro, you can put all the options and their values in a “Configuration file†and tell the programs to read the option values from there. Let’s create a configuration file. In your favorite text editor, make a file named ‘my-cosmology.conf’ (or ‘my-cosmology.txt’, the suffix doesn’t matter) which contains the following lines. One space between the option value and name is enough, the values are just under each other to help in readability. Also note that you can only use long option names in configuration files. H0 70 olambda 0.7 omatter 0.3 You can now tell CosmicCalculator to read this file for option values immediately using the ‘--config’ option as shown below. Do you see how the output of the following command corresponds to the option values in ‘my-cosmology.txt’ (previous command)? $ astcosmiccal --config=my-cosmology.conf -z2 If you need this cosmology every time you are working in a specific directory, you can benefit from Gnuastro’s default configuration files to avoid having to call the ‘--config’ option. Let’s assume that you want any CosmicCalculator call you make in the ‘my-cosmology’ directory to use these parameters. You just have to copy the above configuration file into a special directory and file: $ mkdir my-cosmology $ mkdir my-cosmology/.gnuastro $ mv my-cosmology.conf my-cosmology/.gnuastro/astcosmiccal.conf Once you run CosmicCalculator within ‘my-cosmology’ as shown below, you will see how your cosmology has been implemented without having to type anything extra on the command-line. $ cd my-cosmology $ astcosmiccal -z2 $ cd .. To further simplify the process, you can use the ‘--setdirconf’ option. If you are already in your desired directory, calling this option with the others will automatically write the final values (along with descriptions) in ‘.gnuastro/astcosmiccal.conf’. For example the commands below will make the same configuration file automatically (with one extra call to CosmicCalculator). $ mkdir my-cosmology2 $ cd my-cosmology2 $ astcosmiccal --H0 70 --olambda=0.7 --omatter=0.3 --setdirconf $ astcosmiccal -z2 $ cd .. Gnuastro’s programs also have default configuration files for a specific user (when run in any directory). This allows you to set a special behavior every time a program is run by a specific user. Only the directory and filename differ from the above, the rest of the process is similar to before. Finally, there are also system-wide configuration files that can be used to define the option values for all users on a system. See *note Configuration file precedence:: for a more detailed discussion. We are now ready to start processing the downloaded images. Since these datasets are already aligned, you don’t need to align them to make sure the pixel grid covers the same region in all inputs. Gnuastro’s Warp program has features for such pixel-grid warping (see *note Warp::). Therefore, just for a demonstration, let’s assume one image needs to be rotated by 20 degrees to correspond to the other. To do that, you can run the following command: $ astwarp flat-ir/xdf-f160w.fits --rotate=20 Open the output and see the output. If your final image is already aligned with RA and Dec, you can simply use the ‘--align’ option and let Warp calculate the necessary rotation. Warp can generally be used for any kind of pixel grid manipulation (warping). For example the outputs of the commands below will respectively have larger pixels (new resolution being one quarter the original resolution), get shifted by 2.8 (by sub-pixel), get a shear of 2, and be tilted (projected). After running each, please open the output file and see the effect. $ astwarp flat-ir/xdf-f160w.fits --scale=0.25 $ astwarp flat-ir/xdf-f160w.fits --translate=2.8 $ astwarp flat-ir/xdf-f160w.fits --shear=2 $ astwarp flat-ir/xdf-f160w.fits --project=0.001,0.0005 You can also combine multiple warps in one command. For example to first rotate the image, then scale it, run this command: $ astwarp flat-ir/xdf-f160w.fits --rotate=20 --scale=0.25 If you have multiple warps, do them all in one command. Don’t warp them in separate commands because the correlated noise will become too strong. As you see in the matrix that is printed when you run Warp, it merges all the warps into a single warping matrix (see *note Warping basics:: and *note Merging multiple warpings::) and simply applies that just once. Recall that since this is done through matrix multiplication, order matters in the separate operations. In fact through Warp’s ‘--matrix’ option, you can directly request your desired final warp and don’t have to break it up into different warps like above (see *note Invoking astwarp::). Fortunately these datasets are already aligned to the same pixel grid, so you don’t actually need the files that were just generated. You can safely delete them all with the following command. Here, you see why we put the processed outputs that we need later into a separate directory. In this way, the top directory can be used for temporary files for testing that you can simply delete with a generic command like below. $ rm *.fits To detect the objects in the image, we’ll run NoiseChisel: $ mkdir noisechisel $ astnoisechisel flat-ir/xdf-f160w.fits -onoisechisel/xdf-f160w.fits Read what NoiseChisel writes on the command-line. The curious thing you will notice is that while there were more than 3000 pseudo detections to find the pseudo-detection S/N, but there were only slightly more than 100 clumps to find the false clump S/N. We will see what caused this after a short review on the output of NoiseChisel. NoiseChisel’s output is a single file containing multiple extensions. You can get basic information about the extensions in a FITS file with Gnuastro’s Fits program (see *note Fits::) as shown below. It contains 6 extensions and the first (counted as zero) is blank (has no data). $ astfits noisechisel/xdf-f160w.fits NoiseChisel puts some general information on its outputs in the FITS header of the respective extension. To see the full list of keywords, you can again use the Fits program like above, but also give it your desired extension/HDU. You can also give the extension number (as listed in the output above), for example ‘-h2’ instead of ‘-hOBJECTS’. $ astfits noisechisel/xdf-f160w.fits -hOBJECTS The ‘NUMLABS’ keyword in NoiseChisel’s ‘OBJECTS’ extension contains the number of objects that was found by NoiseChisel in that run. Try to visually find it in the header keywords you saw above. To simplify the process, you can pipe the output of the command above into ‘grep’ (a program for matching lines which is available on almost all Unix-like operating systems). $ astfits noisechisel/xdf-f160w.fits -hOBJECTS | grep NUMLABS If you just want the value of the keyword and not the full FITS keyword line, you can use AWK. In the example below, AWK will print the third word (separated by white space characters) in any line that has a first column value of ‘NUMLABS’. You can also try this for the third HDU (called ‘CLUMPS’) to see the number of clumps. $ astfits noisechisel/xdf-f160w.fits -h2 \ | awk '$1=="NUMLABS" {print $3}' Grep and AWK are simple, but very powerful command-line software for processing text files. Learning them properly can greatly simplify your processing, while improve your creativity, productivity and speed. When you get time, it is highly recommended to master them. The most common implementation of both is from GNU. Like almost all GNU software, both GNU Grep and GNU AWK have wonderful manuals which come with the program for free. You don’t have to read the whole manual at once, they both start with great generic introductions to get you going fast. As described above, you can read both manuals or refresh your memory on your command-line with these commands: $ info awk $ info grep You can now open NoiseChisel’s output with SAO DS9 and visually inspect it. Just note that since there are multiple extensions, the easiest way to view the whole file is to open it as a “Multi-extension data cube†with the ‘-mecube’ option as shown below. If you use GNOME (another GNU software, most common graphic user interface in GNU/Linux operating systems), please see *note Viewing multiextension FITS images:: to open DS9 in multi-extension cube mode by default when using the GUI (double clicking on the file). $ ds9 -mecube noisechisel/xdf-f160w.fits -zscale -zoom to fit Using Gnuastro’s Fits program, you can also copy a HDU from one FITS file to another (for more, see *note HDU manipulation::). So if you want to have a FITS file with only the detected objects, you can run this command: $ astfits noisechisel/xdf-f160w.fits --copy=OBJECTS -oobjects.fits One good way to see if you have missed any signal is to mask all the detected pixels and inspect the noise pixels. For this, you can use Gnuastro’s Arithmetic program (in particular its ‘where’ operator as shown below, see *note Arithmetic operators::). With this command, all input pixels that have a value larger than zero in the ‘OBJECTS’ extension will be set to NaN in the output (written in ‘det-masked.fits’). If you change the ‘gt’ (for “greater thanâ€) operator to ‘eq’ (for “equalâ€), all the un-detected (sky) pixels will be masked and you can see the detections. $ astarithmetic noisechisel/xdf-f160w.fits \ noisechisel/xdf-f160w.fits 0 gt nan where -h1 -h2 \ --output=nc-masked.fits In some cases, you might want to use a different kernel with NoiseChisel (not the default one). To do that, you can use MakeProfiles (see *note MakeProfiles::) in the following manner to build a 2D Gaussian kernel with a FWHM of 3 pixels that extends 5 times the FWHM. This new kernel can later be fed into NoiseChisel with the ‘--kernel’ option. $ astmkprof --kernel=gaussian,3,5 --oversample=1 -okernel-g-3-5.fits $ astnoisechisel flat-ir/xdf-f160w.fits --kernel=kernel-g-3-5.fits \ --output=nc-my-kernel.fits NoiseChisel can produce “Check images†to help you visualize how each step is completed. You can see all the check images it can produce with this command. $ astnoisechisel --help | grep check The check images are also multi-extension FITS files. After each check image is produced, open it with ds9 like NoiseChisel’s output above and flip through the extensions to see each processing in detail. It is _strongly_ encouraged to play with the different parameters and use the respective check images to see which step is affected by your change. The three most useful check images are ‘--checkqthresh’, ‘--checkdetection’, and ‘--checksegmentation’. We can now get back to the curious situation we noticed after running NoiseChisel: the number of false clumps to find an S/N limit was very small (given the extent of this image). This is bad, because we use quantiles in NoiseChisel and such a small number will result in a relatively large scatter. Since this is a segmentation issue, let’s see why this happens with ‘--checksegmentation’. $ astnoisechisel flat-ir/xdf-f160w.fits --checksegmentation To help you get a result faster, when check images are requested, NoiseChisel doesn’t finish its processing (unless you also call ‘--continueaftercheck’). NoiseChisel aborts with an explanation of why it stopped without finishing and the file name of the check image that it produced. The first five extensions are: the input image, the convolved image, the initially labeled detected regions, all the sky region (false) clumps, and those that will be used for S/N. The sky clumps are found over NoiseChisel’s “large tiles†independently. When inspecting the fourth extension of the check image, it is interesting how NoiseChisel has ignored most large tiles and only used the few that we see, mostly on the edge. The reason that almost all internal large tiles are ignored is that galaxies are extended and this is a very deep (and small) image. Thanks to the PSF (see *note PSF::), no object will have a sharp truncation. We have not seen any abrupt break in the light profile of any galaxy: galaxies are always larger when we get deeper datasets. Therefore, in a noisy image, some light will always be left un-detected. To be less affected by this un-detected light, NoiseChisel has the ‘--minskyfrac’ option (see *note General NoiseChisel options::): any tile that has a larger fraction of detected pixels will be ignored. So let’s see what the default value of this option is (recall that with ‘-P’, you can list all the options with their values in Gnuastro’s programs): $ astnoisechisel -P | grep minskyfrac Try decreasing this value and re-running NoiseChisel to see the effect on the fraction of large tiles that will be used for finding false/sky clumps. Play a little with this parameter (give it different values and check the result). $ astnoisechisel flat-ir/xdf-f160w.fits --minskyfrac=0.5 \ --checksegmentation The smaller the value to ‘--minskyfrac’, the more probable that un-detected light in the wings of galaxies will bias/affect the derived false clump S/N. So it is always important to find a good balance between a larger ‘--minskyfrac’ while having a sufficient number of resulting clumps (to avoid scatter). NoiseChisel doesn’t just find the labeled pixels, it also finds the Sky value and the Sky standard deviation in the final two extensions of its output. To generate a catalog of the colors, we will be using the NoiseChisel labeled image from the F160W image. But the Sky and Sky standard deviation values for each different filter will also be necessary. So we’ll run NoiseChisel with our finalized parameters value on both filters (you can also put this option’s value in a configuration file to avoid repeating it). $ astnoisechisel flat-ir/xdf-f105w.fits -onoisechisel/xdf-f105w.fits \ --minskyfrac=0.5 $ astnoisechisel flat-ir/xdf-f160w.fits -onoisechisel/xdf-f160w.fits \ --minskyfrac=0.5 Now, we are ready to make a catalog. We want the object and clump labels from the F160W image. But the input, Sky and Sky standard deviation images should come from each filter. So, we’ll run MakeCatalog on NoiseChisel’s output differently for each filter. When making the F105W catalog, we’ll use the ‘--objectsfile’ and ‘--clumpsfile’ options to tell MakeCatalog to read the object and clump labels from the F160W NoiseChisel output. When these options aren’t given, MakeCatalog will look into the same input file for object and clump labels. For both filters, we’ll ask for the ID, RA, Dec, Magnitude and signal-to-noise ratio (see *note Quantifying measurement limits::). To see a list of all the parameters that MakeCatalog can measure for you, run it with ‘--help’ option. $ mkdir catalog $ astmkcatalog noisechisel/xdf-f160w.fits --zeropoint=25.94 \ --ids --ra --dec --magnitude --sn \ --output=catalog/xdf-f160w.fits $ astmkcatalog noisechisel/xdf-f105w.fits --zeropoint=26.27 \ --objectsfile=noisechisel/xdf-f160w.fits \ --clumpsfile=noisechisel/xdf-f160w.fits \ --ids --ra --dec --magnitude --sn \ --output=catalog/xdf-f105w.fits MakeCatalog can also produce catalogs in plain text format. Please run the MakeCatalog commands above again and replace the ‘.fits’ suffix, in the value to ‘--output’, with ‘.txt’ (we will also be using the text file outputs later). When a clumps image is also given(6), like this example, two catalogs will be made. If you asked for a plain text file output, two files will be made with the ‘_c.txt’ and ‘_o.txt’ suffixes. If MakeCatalog’s output is requested to be FITS, the two catalogs will be in separate extensions of a single file. You can inspect the separate extensions with the Fits program like before (as shown below). Afterwards, you can inspect the table in each extension with Gnuastro’s Table program (see *note Table::) as shown below. $ astfits catalog/xdf-f105w.fits # Extension information $ asttable catalog/xdf-f105w.fits -h1 --info # Objects catalog info. $ asttable catalog/xdf-f105w.fits -h1 # Objects catalog columns. $ asttable catalog/xdf-f105w.fits -h2 -i # Clumps catalog info. $ asttable catalog/xdf-f105w.fits -h2 # Clumps catalog columns. As you see above, to see the column contents of each table, you can just remove the ‘--info’ (or ‘-i’) option. If you want to print the contents of special column(s), just specify the column number(s) (counting from ‘1’, same as output of the command above) or the column name(s) (if they have one). For example, if you just want the objects and clumps magnitude and signal-to-noise ratio in the F160W filter. You can get it with the following commands. $ asttable catalog/xdf-f160w.fits -h1 -cMAGNITUDE -cSN $ asttable catalog/xdf-f160w.fits -h2 -cMAGNITUDE -cSN The clumps catalog has two ID columns (one for the over-all clump ID and one for the ID of the clump in its host object), the magnitude column numbers differ between the object and clumps catalog. So if you want to specify the columns by number, you will need to change the numbers when viewing the clump and objects catalogs. This is a useful advantage of having/using column names. $ asttable catalog/xdf-f160w.fits -h1 -c4 -c5 $ asttable catalog/xdf-f160w.fits -h2 -c5 -c6 Finally, the comments in MakeCatalog’s output (in FITS headers or lines starting with ‘#’ in plain text) contain some important information about the dataset that can be useful. Open ‘catalog/xdf-f160w_o.txt’ in a text editor to see them. Since we used the same labeled image on both filters, the number of rows in both catalogs are the same. So, let’s measure the colors of the objects in this image. We’ll merge the two clump catalogs together into one using the ‘paste’ program on the command-line. The output file will have each line of both catalogs merged into a single line. $ paste catalog/xdf-f160w_c.txt catalog/xdf-f105w_c.txt \ > xdf-f160w-f105w_c_p.txt Open ‘xdf-f160w-f105w_c_p.txt’ after making it to see how ‘paste’ has operated. We can now use AWK to find the colors. We’ll ask AWK to only use lines that don’t start with ‘#’ and don’t have a NaN magnitude in the 9th column (F105W magnitude(7)). We will also ignore columns which don’t have reliable F105W magnitudes (with a S/N less than 7(8)). For the other lines, AWK will print the ID, positional columns and the difference between the respective magnitude columns. $ awk '!/^#/ && $11!="nan" && $12>7 {print $1, $2, $3, $4, $11-$5}' \ xdf-f160w-f105w_c_p.txt > catalog/xdf-f105w-f160w_c.txt Gnuastro has a simple program for basic statistical analysis. The command below will print some basic information about the distribution (minimum, maximum, median and etc), along with a cute little ASCII histogram to visually help you understand the distribution on the command-line without the need for a graphic user interface (see *note Invoking aststatistics::). This ASCII histogram can be useful when you just want some coarse and general information on the input dataset. It is also useful when working on a server (where you may not have graphic user interface), and finally, its fast. $ aststatistics catalog/xdf-f105w-f160w_c.txt -c5 You can later use Gnuastro’s Statistics program with the ‘--histogram’ option to build a much more fine-grained histogram as a table to feed into your favorite plotting program for a much more accurate/appealing plot. If you just want a specific measure, for example the mean, median and standard deviation, you can ask for them specifically: $ aststatistics catalog/xdf-f105w-f160w_c.txt -c5 --mean --median --std Some researchers prefer to have colors in a fixed aperture for all the objects. The colors we calculated above used a different segmentation map for each object. This might not satisfy some science cases. To make a fixed aperture catalog, we should make a labeled image which has a fixed label for each aperture. That labeled image can be given to MakeCatalog instead of NoiseChisel’s labeled detection image. We’ll use the objects catalog in the F160W catalog we generated before for the positions and set the other parameters of each profile to be a fixed circle of radius 5 pixels (we want all apertures to be fixed after all). AWK is a wonderful tool for such jobs as the command below shows. $ awk '!/^#/{print $1, $2, $3, 5, 5, 0, 0, 1, $1, 1}' \ catalog/xdf-f160w_c.txt > catalog/apertures.txt We can now feed this catalog into MakeProfiles to build the apertures for us. See *note Invoking astmkprof:: for a description of the options. The most important for this particular job is ‘--mforflatpix’, it tells MakeProfiles that the values in the magnitude column should be used for each pixel of a flat profile. Without it, MakeProfiles would build the profiles such that the _sum_ of the pixels of each profile would have a _magnitude_ (in log-scale) of the value given in that column (what you would expect when simulating a galaxy for example). $ astmkprof catalog/apertures.txt --background=flat-ir/xdf-f160w.fits \ --clearcanvas --replace --type=int16 --mforflatpix \ --mode=wcs The first thing you might notice in the printed information is that the profiles are not built in order. This is because MakeProfiles works in parallel and parallel CPU operations are asynchronous. Without ‘--replace’, the output is the same in any case. You can try running MakeProfiles with one thread (using ‘--numthreads=1’ to see how order is respected in that case. Open the output ‘apertures.fits’ file and see the result. Where the apertures overlap, you will notice that one label has replaced the other (because of the ‘--replace’ option). In the future, MakeCatalog will be able to work with overlapping labels, but currently it doesn’t. If you are interested, please join us in completing Gnuastro with added improvements like this (see task 14750 (9)). ‘apertures.fits’ labeled image can now be fed input into MakeCatalog. Similar to how we used the F160W labels for the F105W catalog: the labels don’t have to be produced by NoiseChisel. In comparison with the previous MakeCatalog call, notice how 1) we have no more clumps image, 2) that we have set ‘--objectshdu=1’ (since ‘apertures.fits’ is not the output of NoiseChisel where the labeled image is in the third extension), and 3) that we are now using ‘--objid’ instead of ‘--ids’ to avoid warnings that some ID columns are only for clumps. $ astmkcatalog noisechisel/xdf-f105w.fits --zeropoint=26.27 \ --objectsfile=apertures.fits --objectshdu=1 \ --objid --ra --dec --magnitude --sn \ --output=catalog/xdf-f105w-aper.fits Change the filter name and zeropoint magnitudes and run this command again to have the fixed aperture magnitude in the F160W filter also. From this point on, you can follow the previous steps to derive the color in a fixed aperture. We will now find some of the objects with the strongest color difference and make a cutout to inspect them visually: let’s see what the objects with a color more than two magnitudes look like. We’ll use the ‘catalog/xdf-f105w-f160w_c.txt’ file that we produced above. With the command below, all lines with a color value more than 2 will be put in ‘reddest.txt’ and inspect it using ‘cat’. $ awk '$5>1' catalog/xdf-f105w-f160w_c.txt > reddest.txt $ cat reddest.txt We can now feed ‘reddest.txt’ into Gnuastro’s crop to see what these objects look like. To keep things clean, we’ll make a directory called ‘reddest’ and ask Crop to save the crops in this directory. We’ll also add a ‘-f160w.fits’ suffix to the crops. $ mkdir crop $ astcrop --mode=wcs --coordcol=3 --coordcol=4 flat-ir/xdf-f160w.fits \ --catalog=reddest.txt --width=15/3600,15/3600 \ --suffix=-f160w.fits --output=crop Like the MakeProfiles command above, you might notice that the crops aren’t made in order. Since each crop is independent of the rest, the crops are done in parallel and parallel operations are asynchronous. In the command above, change ‘f160w’ to ‘f105w’ to make the crops in both filters. To view the crops more easily (not having to open ds9 for each image), you can convert the FITS crops into the JPEG format. $ for f in *.fits; do \ astconvertt $f --fluxlow=-0.001 --fluxhigh=0.005 --invert -ojpg; \ done The loop above is in series: each file is processed only after the previous ones are complete. If you have GNU Parallel (https://www.gnu.org/software/parallel), you can greatly speed up this conversion. GNU Parallel will run the separate commands simultaneously on different CPU threads in parallel. For more information on efficiently using your threads, see *note Multi-threaded operations::. $ parallel astconvertt --fluxlow=-0.001 --fluxhigh=0.005 --invert \ -ojpg ::: *.fits You can now easily use your general GUI image viewer to flip through the images more easily. On GNOME, you can use the “Eye of GNOME†image viewer (with executable name of ‘eog’). Run the command below and by pressing the <> key, you can flip through the images and compare them visually more easily. Of course, the flux ranges have been chosen generically here for seeing the fainter parts. Therefore, brighter objects will be fully black. $ eog 1-f105w.jpg Another thing that is commonly needed is to visually mark these objects on the image. DS9 has “Regionâ€s for this purpose. You just have to convert your catalog into a “region file†to feed into DS9. To do that, you can use AWK again as shown below. $ cd .. $ awk 'BEGIN{print "# Region file format: DS9 version 4.1"; \ print "global color=green width=2"; \ print "fk5";} \ {printf "circle(%s,%s,1\")\n", $3, $4;}' reddest.txt \ > reddest.reg This region file can be loaded into DS9 with its ‘-regions’ option as shown below (see above for the other options): $ ds9 -mecube noisechisel/xdf-f160w.fits -zscale -zoom to fit \ -regions load all reddest.reg Finally, if this book or any of the programs in Gnuastro have been useful for your research, please cite the respective papers. All Gnuastro programs have a ‘--cite’ option to help you cite the authors’ work more easily. For example: $ astmkcatalog --cite ---------- Footnotes ---------- (1) See *note SAO ds9::, available at . (2) . (3) . (4) GNU Info is already available on almost all Unix-like operating systems. (5) Note that you only have one port to the internet, so downloading in parallel will actually be slower than downloading in series. (6) MakeCatalog will look at the ‘WCLUMPS’ keyword in the objects image to see if it should also use a clumps image or not. (7) Recall that the objects and clumps labels were made on the F160W image. On the F105W image, there might not be enough signal, so random scatter may give a negative total brightness and thus a NaN magnitude. (8) The value of 7 is taken from the clump S/N threshold in F160W (where the clumps were defined). (9)  File: gnuastro.info, Node: Installation, Next: Common program behavior, Prev: Tutorials, Up: Top 3 Installation ************** The latest released version of Gnuastro source code is always available at the following URL: *note Quick start:: describes the commands necessary to configure, build, and install Gnuastro on your system. This chapter will be useful in cases where the simple procedure above is not sufficient, for example your system lacks a mandatory/optional dependency (in other words, you can’t pass the ‘$ ./configure’ step), or you want greater customization, or you want to build and install Gnuastro from other random points in its history, or you want a higher level of control on the installation. Thus if you were happy with downloading the tarball and following *note Quick start::, then you can safely ignore this chapter and come back to it in the future if you need more customization. *note Dependencies:: describes the mandatory, optional and bootstrapping dependencies of Gnuastro. Only the first group are required/mandatory when you are building Gnuastro using a tarball (see *note Release tarball::), they are very basic and low-level tools used in most astronomical software, so you might already have them installed, if not they are very easy to install as described for each. *note Downloading the source:: discusses the two methods you can obtain the source code: as a tarball (a significant snapshot in Gnuastro’s history), or the full history(1). The latter allows you to build Gnuastro at any random point in its history (for example to get bug fixes or new features that are not released as a tarball yet). The building and installation of Gnuastro is heavily customizable, to learn more about them, see *note Build and install::. This section is essentially a thorough explanation of the steps in *note Quick start::. It discusses ways you can influence the building and installation. If you encounter any problems in the installation process, it is probably already explained in *note Known issues::. In *note Other useful software:: the installation and usage of some other free software that are not directly required by Gnuastro but might be useful in conjunction with it is discussed. * Menu: * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. ---------- Footnotes ---------- (1) *note Bootstrapping dependencies:: are required if you clone the full history.  File: gnuastro.info, Node: Dependencies, Next: Downloading the source, Prev: Installation, Up: Installation 3.1 Dependencies ================ The dependencies needed to build and install Gnuastro are defined by the features you want and how you would like to obtain the source code (see *note Downloading the source::). A minimal set of dependencies are mandatory, if they are not present you cannot get passed the configuration step. Such mandatory dependencies are therefore very basic (low-level) tools which are easy to obtain, build and install, see *note Mandatory dependencies:: for a full discussion. If you have the packages of *note Optional dependencies::, Gnuastro will have additional functionality (for example converting FITS images to JPEG or PDF). If you are installing from a tarball as explained in *note Quick start::, you can stop reading after this section. However, if you decided to use the version controlled source instead of the tarball (see *note Version controlled source::), an additional bootstrapping step is required before configuration and its dependencies are explained in *note Bootstrapping dependencies::. * Menu: * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source.  File: gnuastro.info, Node: Mandatory dependencies, Next: Optional dependencies, Prev: Dependencies, Up: Dependencies 3.1.1 Mandatory dependencies ---------------------------- The mandatory Gnuastro dependencies are very basic and low-level tools. They all follow the same basic GNU based build system (like that shown in *note Quick start::), so even if you don’t have them, installing them should be pretty straightforward. In this section we explain each program and any specific note that might be necessary in the installation. The most basic choice is to build the packages from source yourself, instead of relying on your distribution’s package management system. While the latter choice is indeed possible, we recommend that you build these dependencies yourself as discussed below. We will send out notifications in the ‘info-gnuastro’ mailing list, see *note Announcements:: when we find out that these requirements are updated. 1. For each package, Gnuastro might preform better (or require) certain configuration options that your distribution’s package managers didn’t add for you. If present, these configuration options are explained during the installation of each in the sections below. When the proper configuration has not been set, the programs should complain and inform you. 2. Your distribution’s pre-built package might not be the most recent release. 3. For the libraries, they might separate the binary file from the header files, see *note Known issues::. 4. Like any other tool, the science you derive from Gnuastro’s tools highly depend on these lower level dependencies, so generally it is much better to have a close connection with them. By reading their manuals, installing them and staying up to date with changes/bugs in them, your scientific results and understanding will also correspondingly improve. * Menu: * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS.  File: gnuastro.info, Node: GNU Scientific Library, Next: CFITSIO, Prev: Mandatory dependencies, Up: Mandatory dependencies 3.1.1.1 GNU Scientific library .............................. The GNU Scientific Library (http://www.gnu.org/software/gsl/), or GSL, is a large collection of functions that are very useful in scientific applications, for example integration, random number generation, and Fast Fourier Transform among many others. To install GSL from source, you can run the following commands after you have downloaded ‘gsl-latest.tar.gz’ (ftp://ftp.gnu.org/gnu/gsl/gsl-latest.tar.gz): $ tar xf gsl-latest.tar.gz $ cd gsl-X.X # Replace X.X with version number. $ ./configure $ make -j8 # Replace 8 with no. CPU threads. $ make check $ sudo make install  File: gnuastro.info, Node: CFITSIO, Next: WCSLIB, Prev: GNU Scientific Library, Up: Mandatory dependencies 3.1.1.2 CFITSIO ............... CFITSIO (http://heasarc.gsfc.nasa.gov/fitsio/) is the closest you can get to the pixels in a FITS image while remaining faithful to the FITS standard (http://fits.gsfc.nasa.gov/fits_standard.html). It is written by William Pence, the principal author of the FITS standard(1), and is regularly updated. Setting the definitions for all other software packages using FITS images. Some GNU/Linux distributions have CFITSIO in their package managers, if it is available and updated, you can use it. One problem that might occur is that CFITSIO might not be configured with the ‘--enable-reentrant’ option by the distribution. This option allows CFITSIO to open a file in multiple threads, it can thus provide great speed improvements. If CFITSIO was not configured with this option, any program which needs this capability will warn you and abort when you ask for multiple threads (see *note Multi-threaded operations::). To install CFITSIO from source, we strongly recommend that you have a look through Chapter 2 (Creating the CFITSIO library) of the CFITSIO manual and understand the options you can pass to ‘$ ./configure’ (they aren’t too much). This is a very basic package for most astronomical software and it is best that you configure it nicely with your system. Once you download the source and unpack it, the following configure script should be enough for most purposes. Don’t forget to read chapter two of the manual though, for example the second option is only for 64bit systems. The manual also explains how to check if it has been installed correctly. CFITSIO comes with two executables called fpack and funpack. From their manual: they “are standalone programs for compressing and uncompressing images and tables that are stored in the FITS (Flexible Image Transport System) data format. They are analogous to the gzip and gunzip compression programs except that they are optimized for the types of astronomical images that are often stored in FITS formatâ€. The commands below will compile and install them on your system along with CFITSIO. They are not essential for Gnuastro, since they are just wrappers for functions within CFITSIO, but they can come in handy. The ‘make utils’ command is only available for versions above 3.39, it will build these executables along with several other test executables which are deleted before the installation (otherwise they will also be installed). The CFITSIO installation from source process is given below. Let’s assume you have downloaded ‘cfitsio_latest.tar.gz’ (http://heasarc.gsfc.nasa.gov/FTP/software/fitsio/c/cfitsio_latest.tar.gz) and are in the same directory: $ tar xf cfitsio_latest.tar.gz $ cd cfitsio $ ./configure --prefix=/usr/local --enable-sse2 --enable-reentrant $ make $ make utils $ ./testprog > testprog.lis $ diff testprog.lis testprog.out # Should have no output $ cmp testprog.fit testprog.std # Should have no output $ rm cookbook fitscopy imcopy smem speed testprog $ sudo make install ---------- Footnotes ---------- (1) Pence, W.D. et al. Definition of the Flexible Image Transport System (FITS), version 3.0. (2010) Astronomy and Astrophysics, Volume 524, id.A42, 40 pp.  File: gnuastro.info, Node: WCSLIB, Prev: CFITSIO, Up: Mandatory dependencies 3.1.1.3 WCSLIB .............. WCSLIB (http://www.atnf.csiro.au/people/mcalabre/WCS/) is written and maintained by one of the authors of the World Coordinate System (WCS) definition in the FITS standard (http://fits.gsfc.nasa.gov/fits_standard.html)(1), Mark Calabretta. It might be already built and ready in your distribution’s package management system. However, here the installation from source is explained, for the advantages of installation from source please see *note Mandatory dependencies::. To install WCSLIB you will need to have CFITSIO already installed, see *note CFITSIO::. WCSLIB also has plotting capabilities which use PGPLOT (a plotting library for C). If you wan to use those capabilities in WCSLIB, *note PGPLOT:: provides the PGPLOT installation instructions. However PGPLOT is old(2), so its installation is not easy, there are also many great modern WCS plotting tools (mostly in written in Python). Hence, if you will not be using those plotting functions in WCSLIB, you can configure it with the ‘--without-pgplot’ option as shown below. Let’s assume you have downloaded ‘wcslib.tar.bz2’ (ftp://ftp.atnf.csiro.au/pub/software/wcslib/wcslib.tar.bz2) and are in the same directory: $ tar xf wcslib.tar.bz2 $ cd wcslib-X.X # Replace X.X with version number $ ./configure --without-pgplot LIBS="-pthread -lm" --disable-fortran $ make $ make check $ sudo make install ---------- Footnotes ---------- (1) Greisen E.W., Calabretta M.R. (2002) Representation of world coordinates in FITS. Astronomy and Astrophysics, 395, 1061-1075. (2) As of early June 2016, its most recent version was uploaded in February 2001.  File: gnuastro.info, Node: Optional dependencies, Next: Bootstrapping dependencies, Prev: Mandatory dependencies, Up: Dependencies 3.1.2 Optional dependencies --------------------------- The libraries listed here are only used for very specific applications, therefore if you don’t want these operations, Gnuastro will be built and installed without them and you don’t have to have the dependencies. If the ‘./configure’ script can’t find these requirements, it will warn you in the end that they are not present and notify you of the operation(s) you can’t do due to not having them. If the output you request from a program requires a missing library, that program is going to warn you and abort. In the case of executables like GPL GhostScript, if you install them at a later time, the program will run. This is because if required libraries are not present at build time, the executables cannot be built, but an executable is called by the built program at run time so if it becomes available, it will be used. If you do install an optional library later, you will have to rebuild Gnuastro and reinstall it for it to take effect. GNU Libtool Libtool is a program to simplify managing of the libraries to build an executable (a program). GNU Libtool has some added functionality compared to other implementations. If GNU Libtool isn’t present on your system at configuration time a warning will be printed and *note BuildProgram:: won’t be built or installed. The configure script will look into your search path (‘PATH’) for GNU Libtool through the following executable names: ‘libtool’ (acceptable only if it is the GNU implementation) or ‘glibtool’. See *note Installation directory:: for more on ‘PATH’. GNU Libtool (the binary/executable file) is a low-level program that is probably already present on your system, and if not, is available in your operating system package manager(1). If you want to install GNU Libtool’s latest version from source, please visit its webpage (https://www.gnu.org/software/libtool/). Gnuastro’s tarball is shipped with an internal implementation of GNU Libtool. Even if you have GNU Libtool, Gnuastro’s internal implementation is used for the building and installation of Gnuastro. As a result, you can still build, install and use Gnuastro even if you don’t have GNU Libtool installed on your system. However, this internal Libtool does not get installed. Therefore, after Gnuastro’s installation, if you want to use *note BuildProgram:: to compile and link your own C source code which uses the *note Gnuastro library::, you need to have GNU Libtool available on your system (independent of Gnuastro). See *note Review of library fundamentals:: to learn more about libraries. libgit2 Git is one of the most common version control systems (see *note Version controlled source::). When ‘libgit2’ is present, and Gnuastro’s programs are run within a version controlled directory, outputs will contain the version number of the working directory’s repository for future reproducibility. See the ‘COMMIT’ keyword header in *note Output headers:: for a discussion. libjpeg libjpeg is only used by ConvertType to read from and write to JPEG images. libjpeg (http://www.ijg.org/) is a very basic library that provides tools to read and write JPEG images, most of the GNU/Linux graphic programs and libraries use it. Therefore you most probably already have it installed. libjpeg-turbo (http://libjpeg-turbo.virtualgl.org/) is an alternative to libjpeg. It uses SIMD instructions for ARM based systems that significantly decreases the processing time of JPEG compression and decompression algorithms. GPL Ghostscript GPL Ghostscript’s executable (‘gs’) is called used by ConvertType to compile a PDF file from a source PostScript file, see *note ConvertType::. Therefore its headers (and libraries) are not needed. With a very high probability you already have it in your GNU/Linux distribution. Unfortunately it does not follow the standard GNU build style so installing it is very hard. It is best to rely on your distribution’s package managers for this. ---------- Footnotes ---------- (1) Note that we want the binary/executable Libtool program which can be run on the command-line. In Debian-based operating systems which separate various parts of a package, you want want ‘libtool-bin’, the ‘libtool’ package won’t contain the executable program.  File: gnuastro.info, Node: Bootstrapping dependencies, Prev: Optional dependencies, Up: Dependencies 3.1.3 Bootstrapping dependencies -------------------------------- Bootstrapping is only necessary if you have decided to obtain the full version controlled history of Gnuastro, see *note Version controlled source:: and *note Bootstrapping::. Using the version controlled source enables you to always be up to date with the most recent development work of Gnuastro (bug fixes, new functionalities, improved algorithms and etc). If you have downloaded a tarball (see *note Downloading the source::), then you can ignore this subsection. To successfully run the bootstrapping process, there are some additional dependencies to those discussed in the previous subsections. These are low level tools that are used by a large collection of Unix-like operating systems programs, therefore they are most probably already available in your system. If they are not already installed, you should be able to easily find them in any GNU/Linux distribution package management system (‘apt-get’, ‘yum’, ‘pacman’ and etc). The short names in parenthesis in ‘typewriter’ font after the package name can be used to search for them in your package manager. For the GNU Portability Library, GNU Autoconf Archive and TeX Live, it is recommended to use the instructions here, not your operating system’s package manager. GNU Portability Library (Gnulib) To ensure portability for a wider range of operating systems (those that don’t include GNU C library, namely glibc), Gnuastro depends on the GNU portability library, or Gnulib. Gnulib keeps a copy of all the functions in glibc, implemented (as much as possible) to be portable to other operating systems. The ‘bootstrap’ script can automatically clone Gnulib (as a ‘gnulib/’ directory inside Gnuastro), however, as described in *note Bootstrapping:: this is not recommended. The recommended way to bootstrap Gnuastro is to first clone Gnulib and the Autoconf archives (see below) into a local directory outside of Gnuastro. Let’s call it ‘DEVDIR’(1) (which you can set to any directory). Currently in Gnuastro, both Gnulib and Autoconf archives have to be cloned in the same top directory(2) like the case here(3): $ DEVDIR=/home/yourname/Development $ cd $DEVDIR $ git clone git://git.sv.gnu.org/gnulib.git $ git clone git://git.sv.gnu.org/autoconf-archive.git You now have the full version controlled source of these two repositories in separate directories. Both these packages are regularly updated, so every once in a while, you can run ‘$ git pull’ within them to get any possible updates. GNU Automake (‘automake’) GNU Automake will build the ‘Makefile.in’ files in each sub-directory using the (hand-written) ‘Makefile.am’ files. The ‘Makefile.in’s are subsequently used to generate the ‘Makefile’s when the user runs ‘./configure’ before building. GNU Autoconf (‘autoconf’) GNU Autoconf will build the ‘configure’ script using the configurations we have defined (hand-written) in ‘configure.ac’. GNU Autoconf Archive These are a large collection of tests that can be called to run at ‘./configure’ time. See the explanation under GNU Portability Library above for instructions on obtaining it and keeping it up to date. GNU Libtool (‘libtool’) GNU Libtool is in charge of building all the libraries in Gnuastro. The libraries contain functions that are used by more than one program and are installed for use in other programs. They are thus put in a separate directory (‘lib/’). GNU help2man (‘help2man’) GNU help2man is used to convert the output of the ‘--help’ option (*note --help::) to the traditional Man page (*note Man pages::). LaTeX and some TeX packages Some of the figures in this book are built by LaTeX (using the PGF/TikZ package). The LaTeX source for those figures is version controlled for easy maintenance not the actual figures. So the ‘./boostrap’ script will run LaTeX to build the figures. The best way to install LaTeX and all the necessary packages is through TeX live (https://www.tug.org/texlive/) which is a package manager for TeX related tools that is independent of any operating system. It is thus preferred to the TeX Live versions distributed by your operating system. To install TeX Live, go to the webpage and download the appropriate installer by following the “download†link. Note that by default the full package repository will be downloaded and installed (around 4 Giga Bytes) which can take _very_ long to download and to update later. However, most packages are not needed by everyone, it is easier, faster and better to install only the “Basic scheme†(consisting of only the most basic TeX and LaTeX packages, which is less than 200 Mega bytes)(4). After the installation, be sure to set the environment variables as suggested in the end of the outputs. Any time you confront (need) a package you don’t have, simply install it with a command like below (similar to how you install software from your operating system’s package manager)(5). To install all the necessary TeX packages for a successful Gnuastro bootstrap, run this command: $ su # tlmgr install epsf jknapltx caption biblatex biber iftex \ etoolbox logreq xstring xkeyval pgf ms \ xcolor pgfplots times rsfs pstools epspdf ImageMagick (‘imagemagick’) ImageMagick is a wonderful and robust program for image manipulation on the command-line. ‘bootsrap’ uses it to convert the book images into the formats necessary for the various book formats. ---------- Footnotes ---------- (1) If you are not a developer in Gnulib or Autoconf archives, ‘DEVDIR’ can be a directory that you don’t backup. In this way the large number of files in these projects won’t slow down your backup process or take bandwidth (if you backup to a remote server). (2) If you already have the Autoconf archives in a separate directory, or can’t clone it in the same directory as Gnulib, or you have it with another directory name (not ‘autoconf-archive/’), you can follow this short step. Set ‘AUTOCONFARCHIVES’ to your desired address. Then define a symbolic link in ‘DEVDIR’ with the following command so Gnuastro’s bootstrap script can find it: ‘$ ln -s $AUTOCONFARCHIVES $DEVDIR/autoconf-archive’. (3) If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the git protocol. In that case use the following URL for the HTTP protocol instead (for Autoconf archives, replace the name): ‘http://git.sv.gnu.org/r/gnulib.git’ (4) You can also download the DVD iso file at a later time to keep as a backup for when you don’t have internet connection if you need a package. (5) After running TeX, or LaTeX, you might get a warning complaining about a ‘missingfile’. Run ‘‘tlmgr info missingfile’’ to see the package(s) containing that file which you can install.  File: gnuastro.info, Node: Downloading the source, Next: Build and install, Prev: Dependencies, Up: Installation 3.2 Downloading the source ========================== Gnuastro’s source code can be downloaded in two ways. As a tarball, ready to be configured and installed on your system (as described in *note Quick start::), see *note Release tarball::. If you want official releases of stable versions this is the best, easiest and most common option. Alternatively, you can clone the version controlled history of Gnuastro, run one extra bootstrapping step and then follow the same steps as the tarball. This will give you access to all the most recent work that will be included in the next release along with the full project history. The process is thoroughly introduced in *note Version controlled source::. * Menu: * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source.  File: gnuastro.info, Node: Release tarball, Next: Version controlled source, Prev: Downloading the source, Up: Downloading the source 3.2.1 Release tarball --------------------- A release tarball (commonly compressed) is the most common way of obtaining free and open source software. A tarball is a snapshot of one particular moment in the Gnuastro development history along with all the necessary files to configure, build, and install Gnuastro easily (see *note Quick start::). It is very straightforward and needs the least set of dependencies (see *note Mandatory dependencies::). Gnuastro has tarballs for official stable releases and pre-releases for testing. See *note Version numbering:: for more on the two types of releases and the formats of the version numbers. The URLs for each type of release are given below. Official stable releases (): This URL hosts the official stable releases of Gnuastro. Always use the most recent version (see *note Version numbering::). By clicking on the “Last modified†title of the second column, the files will be sorted by their date which you can also use to find the latest version. It is recommended to use a mirror to download these tarballs, please visit and see below. Pre-release tar-balls (): This URL contains unofficial pre-release versions of Gnuastro. The pre-release versions of Gnuastro here are for enthusiasts to try out before an official release. If there are problems, or bugs then the testers will inform the developers to fix before the next official release. See *note Version numbering:: to understand how the version numbers here are formatted. If you want to remain even more up-to-date with the developing activities, please clone the version controlled source as described in *note Version controlled source::. Gnuastro’s official/stable tarball is released with two formats: Gzip (with suffix ‘.tar.gz’) and Lzip (with suffix ‘.tar.lz’). The pre-release tarballs (after version 0.3) are released only as an Lzip tarball. Gzip is a very well-known and widely used compression program created by GNU and available in most systems. However, Lzip provides a better compression ratio and more robust archival capacity. For example Gnuastro 0.3’s tarball was 2.9MB and 4.3MB with Lzip and Gzip respectively, see the Lzip webpage (http://www.nongnu.org/lzip/lzip.html) for more. Lzip might not be pre-installed in your operating system, if so, installing it from your operating system’s package manager or from source is very easy and fast (it is a very small program). The GNU FTP server is mirrored (has backups) in various locations on the globe (). You can use the closest mirror to your location for a more faster download. Note that only some mirrors keep track of the pre-release (alpha) tarballs. Also note that if you want to download immediately after and announcement (see *note Announcements::), the mirrors might need some time to synchronize with the main GNU FTP server.  File: gnuastro.info, Node: Version controlled source, Prev: Release tarball, Up: Downloading the source 3.2.2 Version controlled source ------------------------------- The publicly distributed Gnuastro tar-ball (for example ‘gnuastro-X.X.tar.gz’) does not contain the revision history, it is only a snapshot of the source code at one significant instant of Gnuastro’s history (specified by the version number, see *note Version numbering::), ready to be configured and built. To be able to develop successfully, the revision history of the code can be very useful to track when something was added or changed, also some updates that are not yet officially released might be in it. We use Git for the version control of Gnuastro. For those who are not familiar with it, we recommend the Pro Git(1) book. The whole book is publicly available for online reading and downloading and does a wonderful job at explaining the concepts and best practices. Let’s assume you want to keep Gnuastro in the ‘TOPGNUASTRO’ directory (can be any directory, change the value below). The full version controlled history of Gnuastro can be cloned in ‘TOPGNUASTRO/gnuastro’ by running the following commands(2): $ TOPGNUASTRO=/home/yourname/Research/projects/ $ cd $TOPGNUASTRO $ git clone git://git.sv.gnu.org/gnuastro.git The ‘$TOPGNUASTRO/gnuastro’ directory will contain hand-written (version controlled) source code for Gnuastro’s programs, libraries, this book and the tests. All are divided into sub-directories with standard and very descriptive names. The version controlled files in the top cloned directory are either mainly in capital letters (for example ‘THANKS’ and ‘README’) or mainly written in small-caps (for example ‘configure.ac’ and ‘Makefile.am’). The former are non-programming, standard writing for human readers containing high-level information about the whole package. The latter are instructions to customize the GNU build system for Gnuastro. The cloned Gnuastro source cannot immediately be configured, compiled, or installed since it only contains hand-written files, not automatically generated or imported files which do all the hard work of the build process. See *note Bootstrapping:: for the process of generating and importing those files (it is very easy!). Once you have bootstrapped Gnuastro, you can run the standard procedures (in *note Quick start::). Very soon after you have cloned it, Gnuastro’s main ‘master’ branch will be updated on the main repository (since the developers are actively working on Gnuastro), for the best practices in keeping your local history in sync with the main repository see *note Synchronizing::. * Menu: * Bootstrapping:: Adding all the automatically generated files. * Synchronizing:: Keep your local clone up to date. ---------- Footnotes ---------- (1) (2) If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the Git protocol. In that case use the following URL which uses the HTTP protocol instead: ‘http://git.sv.gnu.org/r/gnuastro.git’  File: gnuastro.info, Node: Bootstrapping, Next: Synchronizing, Prev: Version controlled source, Up: Version controlled source 3.2.2.1 Bootstrapping ..................... The version controlled source code lacks the source files that we have not written or are automatically built. These automatically generated files are included in the distributed tar ball for each distribution (for example ‘gnuastro-X.X.tar.gz’, see *note Version numbering::) and make it easy to immediately configure, build, and install Gnuastro. However from the perspective of version control, they are just bloatware and sources of confusion (since they are not changed by Gnuastro developers). The process of automatically building and importing necessary files into the cloned directory is known as _bootstrapping_. All the instructions for an automatic bootstrapping are available in ‘bootstrap’ and configured using ‘bootstrap.conf’. ‘bootstrap’ is the only file not written by Gnuastro developers but is under version control to enable simple bootstrapping immediately after cloning. It is maintained by the GNU Portability Library (Gnulib) and this file is an identical copy, so do not make any changes in this file since it will be replaced when Gnulib releases an update. Make all your changes in ‘bootstrap.conf’. The bootstrapping process has its own separate set of dependencies, the full list is given in *note Bootstrapping dependencies::. They are generally very low-level and used by a very large set of commonly used programs, so they are probably already installed on your system. The simplest way to bootstrap Gnuastro is to simply run the bootstrap script within your cloned Gnuastro directory as shown below. However, please read the next paragraph before doing so (see *note Version controlled source:: for ‘TOPGNUASTRO’). $ cd TOPGNUASTRO/gnuastro $ ./bootstrap # Requires internet connection Without any options, ‘bootstrap’ will clone Gnulib within your cloned Gnuastro directory (‘TOPGNUASTRO/gnuastro/gnulib’) and download the necessary Autoconf archives macros. So if you run bootstrap like this, you will need an internet connection every time you decide to bootstrap. Also, Gnulib is a large package and cloning it can be slow. It will also keep the full Gnulib repository within your Gnuastro repository, so if another one of your projects also needs Gnulib, and you insist on running bootstrap like this, you will have two copies. In case you regularly backup your important files, Gnulib will also slow down the backup process. Therefore while the simple invocation above can be used with no problem, it is not recommended. To do better, see the next paragraph. The recommended way to get these two packages is thoroughly discussed in *note Bootstrapping dependencies:: (in short: clone them in the separate ‘DEVDIR/’ directory). The following commands will take you into the cloned Gnuastro directory and run the ‘bootstrap’ script, while telling it to copy some files (instead of making symbolic links, with the ‘--copy’ option, this is not mandatory(1)) and where to look for Gnulib (with the ‘--gnulib-srcdir’ option). Please note that the address given to ‘--gnulib-srcdir’ has to be an absolute address (so don’t use ‘~’ or ‘../’ for example). $ cd $TOPGNUASTRO/gnuastro $ ./bootstrap --copy --gnulib-srcdir=$DEVDIR/gnulib Since Gnulib and Autoconf archives are now available in your local directories, you don’t need an internet connection every time you decide to remove all untracked files and redo the bootstrap (see box below). You can also use the same command on any other project that uses Gnulib. All the necessary GNU C library functions, Autoconf macros and Automake inputs are now available along with the book figures. The standard GNU build system (*note Quick start::) will do the rest of the job. *Undoing the bootstrap:* During the development, it might happen that you want to remove all the automatically generated and imported files. In other words, you might want to reverse the bootstrap process. Fortunately Git has a good program for this job: ‘git clean’. Run the following command and every file that is not version controlled will be removed. git clean -fxd It is best to commit any recent change before running this command. You might have created new files since the last commit and if they haven’t been committed, they will all be gone forever (using ‘rm’). To get a list of the non-version controlled files instead of deleting them, add the ‘n’ option to ‘git clean’, so it becomes ‘-fxdn’. Besides the ‘bootstrap’ and ‘bootstrap.conf’, the ‘bootstrapped/’ directory and ‘README-hacking’ file are also related to the bootstrapping process. The former hosts all the imported (bootstrapped) directories. Thus, in the version controlled source, it only contains a ‘REAME’ file, but in the distributed tar-ball it also contains sub-directories filled with all bootstrapped files. ‘README-hacking’ contains a summary of the bootstrapping process discussed in this section. It is a necessary reference when you haven’t built this book yet. It is thus not distributed in the Gnuastro tarball. ---------- Footnotes ---------- (1) The ‘--copy’ option is recommended because some backup systems might do strange things with symbolic links.  File: gnuastro.info, Node: Synchronizing, Prev: Bootstrapping, Up: Version controlled source 3.2.2.2 Synchronizing ..................... The bootstrapping script (see *note Bootstrapping::) is not regularly needed: you mainly need it after you have cloned Gnuastro (once) and whenever you want to re-import the files from Gnulib, or Autoconf archives(1) (not too common). However, Gnuastro developers are constantly working on Gnuastro and are pushing their changes to the official repository. Therefore, your local Gnuastro clone will soon be out-dated. Gnuastro has two mailing lists dedicated to its developing activities (see *note Developing mailing lists::). Subscribing to them can help you decide when to synchronize with the official repository. To pull all the most recent work in Gnuastro, run the following command from the top Gnuastro directory: $ git pull && autoconf -f GNU Autoconf is part of the GNU build system and will update the ‘./configure’ script based on the hand-written configurations (in ‘configure.ac’, which is version controlled in Gnuastro). The pulled changes might contain changes in the build system configurations. However, The most important reason for running this command is to generate a version number for your Gnuastro snapshot. This generated version number will include the commit information if you are building Gnuastro from any point in Gnuastro’s history (see *note Version numbering::). Since the version number is included in nearly all outputs of the programs, this can help you later exactly reproduce an old result by checking out the exact point in Gnuastro’s history that produced those results. Therefore, be sure to run ‘‘autoconf -f’’ after every synchronization. You can also run them separately: $ git pull $ autoconf -f If you would like to see what has changed since you last synchronized your local clone, you can take the following steps instead of the simple command above (don’t type anything after ‘#’): $ git checkout master # Confirm if you are on master. $ git fetch origin # Fetch all new commits from server. $ git log master..origin/master # See all the new commit messages. $ git merge origin/master # Update your master branch. $ autoconf -f # Update ./configure. By default ‘git log’ prints the most recent commit first, add the ‘--reverse’ option to see the changes chronologically. To see exactly what has been changed in the source code along with the commit message, add a ‘-p’ option to the ‘git log’. If you intend make changes in the code, have a look at *note Developing:: to get started easily. Be sure to commit your changes in a separate branch (keep your ‘master’ branch to follow the official repository) and re-run ‘autoconf -f’ after the commit. If you intend to send your changes to us (see *note Contributing to Gnuastro::) for the benefit of the whole community. If you send your work to us, you can safely use your commit since it will be ultimately recorded in Gnuastro’s official history. If not, please upload your separate branch to a public hosting service (for example GitLab, see *note Forking tutorial::) and link to it in your report, or run ‘make distcheck’ and upload the output ‘gnuastro-X.X.X.XXXX.tar.gz’ to a publicly accessible webpage so your results can be considered scientific (reproducible). ---------- Footnotes ---------- (1) is defined for you to check if significant (for Gnuastro) updates are made in these repositories, since the last time you pulled from them.  File: gnuastro.info, Node: Build and install, Prev: Downloading the source, Up: Installation 3.3 Build and install ===================== This section is basically a longer explanation to the sequence of commands given in *note Quick start::. If you didn’t have any problems during the *note Quick start:: steps, you want to have all the programs of Gnuastro installed in your system, you don’t want to change the executable names during or after installation, you have root access to install the programs in the default system wide directory, the Letter paper size of the print book is fine for you or as a summary you don’t feel like going into the details when everything is working, you can safely skip this section. If you have any of the above problems or you want to understand the details for a better control over your build and install, read along. The dependencies which you will need prior to configuring, building and installing Gnuastro are explained in *note Dependencies::. The first three steps in *note Quick start:: need no extra explanation, so we will skip them and start with an explanation of Gnuastro specific configuration options and a discussion on the installation directory in *note Configuring::, followed by some smaller subsections: *note Tests::, *note A4 print book::, and *note Known issues:: which explains the solutions to known problems you might encounter in the installation steps and ways you can solve them. * Menu: * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter.  File: gnuastro.info, Node: Configuring, Next: Tests, Prev: Build and install, Up: Build and install 3.3.1 Configuring ----------------- The ‘$ ./configure’ step is the most important step in the build and install process. All the required packages, libraries, headers and environment variables are checked in this step. The behaviors of make and make install can also be set through command line options to this command. The configure script accepts various arguments and options which enable the final user to highly customize whatever she is building. The options to configure are generally very similar to normal program options explained in *note Arguments and options::. Similar to all GNU programs, you can get a full list of the options along with a short explanation by running $ ./configure --help A complete explanation is also included in the ‘INSTALL’ file. Note that this file was written by the authors of GNU Autoconf (which builds the ‘configure’ script), therefore it is common for all programs which use the ‘$ ./configure’ script for building and installing, not just Gnuastro. Here we only discuss cases where you don’t have super-user access to the system and if you want to change the executable names. But before that, a review of the options to configure that are particular to Gnuastro are discussed. * Menu: * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source.  File: gnuastro.info, Node: Gnuastro configure options, Next: Installation directory, Prev: Configuring, Up: Configuring 3.3.1.1 Gnuastro configure options .................................. Most of the options to configure (which are to do with building) are similar for every program which uses this script. Here the options that are particular to Gnuastro are discussed. The next topics explain the usage of other configure options which can be applied to any program using the GNU build system (through the configure script). ‘--enable-progname’ Only build and install ‘progname’ along with any other program that is enabled in this fashion. ‘progname’ is the name of the executable without the ‘ast’, for example ‘crop’ for Crop (with the executable name of ‘astcrop’). If this option is called for any of the programs in Gnuastro, any program which is not explicitly enabled will not be built or installed. ‘--disable-progname’ ‘--enable-progname=no’ Do not build or install the program named ‘progname’. This is very similar to the ‘--enable-progname’, but will build and install all the other programs except this one. ‘--enable-gnulibcheck’ Enable checks on the GNU Portability Library (Gnulib). Gnulib is used by Gnuastro to enable users of non-GNU based operating systems (that don’t use GNU C library or glibc) to compile and use the advanced features that this library provides. We make extensive use of such functions. If you give this option to ‘$ ./configure’, when you run ‘$ make check’, first the functions in Gnulib will be tested, then the Gnuastro executables. If your operating system does not support glibc or has an older version of it and you have problems in the build process (‘$ make’), you can give this flag to configure to see if the problem is caused by Gnulib not supporting your operating system or Gnuastro, see *note Known issues::. ‘--disable-guide-message’ ‘--enable-guide-message=no’ Do not print a guiding message during the GNU Build process of *note Quick start::. By default, after each step, a message is printed guiding the user what the next command should be. Therefore, after ‘./configure’, it will suggest running ‘make’. After ‘make’, it will suggest running ‘make check’ and so on. If Gnuastro is configured with this option, for example $ ./configure --disable-guide-message Then these messages will not be printed after any step (like most programs). For people who are not yet fully accustomed to this build system, these guidelines can be very useful and encouraging. However, if you find those messages annoying, use this option. *Note:* If some programs are enabled and some are disabled, it is equivalent to simply enabling those that were enabled. Listing the disabled programs is redundant. The tests of some programs might depend on the outputs of the tests of other programs. For example MakeProfiles is one the first programs to be tested when you run ‘$ make check’. MakeProfiles’ test outputs (FITS images) are inputs to many other programs (which in turn provide inputs for other programs). Therefore, if you don’t install MakeProfiles for example, the tests for many the other programs will be skipped. To avoid this, in one run, you can install all the programs and run the tests but not install. If everything is working correctly, you can run configure again with only the programs you want. However, don’t run the tests and directly install after building.  File: gnuastro.info, Node: Installation directory, Next: Executable names, Prev: Gnuastro configure options, Up: Configuring 3.3.1.2 Installation directory .............................. One of the most commonly used options to ‘./configure’ is ‘--prefix’, it is used to define the directory that will host all the installed files (or the “prefix†in their final absolute file name). For example, when you are using a server and you don’t have administrator or root access. In this example scenario, if you don’t use the ‘--prefix’ option, you won’t be able to install the built files and thus access them from anywhere without having to worry about where they are installed. However, once you prepare your startup file to look into the proper place (as discussed thoroughly below), you will be able to easily use this option and benefit from any software you want to install without having to ask the system administrators or install and use a different version of a software that is already installed on the server. The most basic way to run an executable is to explicitly write its full file name (including all the directory information) and run it. One example is running the configuration script with the ‘$ ./configure’ command (see *note Quick start::). By giving a specific directory (the current directory or ‘./’), we are explicitly telling the shell to look in the current directory for an executable file named ‘‘configure’’. Directly specifying the directory is thus useful for executables in the current (or nearby) directories. However, when the program (an executable file) is to be used a lot, specifying all those directories will become a significant burden. For example, the ‘ls’ executable lists the contents in a given directory and it is (usually) installed in the ‘/usr/bin/’ directory by the operating system maintainers. So each time you want to use it you would have to run the following command (which is very inconvenient, both in writing and in remembering the various directories). $ /usr/bin/ls To address this problem, we have the ‘PATH’ environment variable. To understand it better, we will start with a short introduction to the shell variables. Shell variable values are basically treated as strings of characters. For example, it doesn’t matter if the value is a name (string of _alphabetic_ characters) or a number (string of _numeric_ characters). You can define a variable and a value for it by running $ myvariable1=a_test_value $ myvariable2="a test value" As you see above, if the value contains white space characters, you have to put the whole value (including white space characters) in double quotes (<">). You can see the value it represents by running $ echo $myvariable1 $ echo $myvariable2 If a variable has no value or it wasn’t defined, the last command will only print an empty line. A variable defined like this will be known as long as this shell or terminal is running. Other terminals will have no idea it existed. The main advantage of shell variables is that if they are exported(1), subsequent programs that are run within that shell can access their value. So by changing their value, you can change the “environment†of a program which uses them. The shell variables which are accessed by programs are therefore known as “environment variablesâ€(2). You can see the full list of exported variables that your shell recognizes by running: $ printenv ‘HOME’ is one commonly used environment variable, it is any user’s (the one that is logged in) top directory. Try finding it in the command above. It is used so often that the shell has a special expansion (alternative) for it: ‘‘~’’. Whenever you see file names starting with the tilde sign, it actually represents the value to the ‘HOME’ environment variable, so ‘~/doc’ is the same as ‘$HOME/doc’. Another one of the most commonly used environment variables is ‘PATH’, it is a list of directories to search for executable names. Its value is a list of directories (separated by a colon, or ‘<:>’). When the address of the executable is not explicitly given (like ‘./configure’ above), the system will look for the executable in the directories specified by ‘PATH’. If you have a computer nearby, try running the following command to see which directories your system will look into when it is searching for executable (binary) files, one example is printed here (notice how ‘/usr/bin’, in the ‘ls’ example above, is one of the directories in ‘PATH’): $ echo $PATH /usr/local/sbin:/usr/local/bin:/usr/bin By default ‘PATH’ usually contains system-wide directories, which are readable (but not writable) by all users, like the above example. Therefore if you don’t have root (or administrator) access, you need to add another directory to ‘PATH’ which you actually have write access to. The standard directory where you can keep installed files (not just executables) for your own user is the ‘~/.local/’ directory. The names of hidden files start with a ‘<.>’ (dot), so it will not show up in your common command-line listings, or on the graphical user interface. You can use any other directory, but this is the most recognized. The top installation directory will be used to keep all the package’s components: programs (executables), libraries, include (header) files, shared data (like manuals), or configuration files (see *note Review of library fundamentals:: for a thorough introduction to headers and linking). So it commonly has some of the following sub-directories for each class of installed components respectively: ‘bin/’, ‘lib/’, ‘include/’ ‘man/’, ‘share/’, ‘etc/’. Since the ‘PATH’ variable is only used for executables, you can add the ‘~/.local/bin’ directory (which keeps the executables/programs or more generally, “binary†files) to ‘PATH’ with the following command. As defined below, first the existing value of ‘PATH’ is used, then your given directory is added to its end and the combined value is put back in ‘PATH’ (run ‘‘$ echo $PATH’’ afterwards to check if it was added). $ PATH=$PATH:~/.local/bin Any executable that you installed in ‘~/.local/bin’ will now be usable without having to remember and write its full address. However, as soon as you leave/close your current terminal session, this modified ‘PATH’ variable will be forgotten. Adding the directories which contain executables to the ‘PATH’ environment variable each time you start a terminal is also very inconvenient and prone to errors. Fortunately, there are standard ‘startup files’ defined by your shell precisely for this (and other) purposes. There is a special startup file for every significant starting step: ‘/etc/profile’ and everything in ‘/etc/profile.d/’ These startup scripts are called when your whole system starts (for example after you turn on your computer). Therefore you need administrator or root privileges to access or modify them. ‘~/.bash_profile’ If you are using (GNU) Bash as your shell, the commands in this file are run once every time you log in to your account. ‘~/.bashrc’ If you are using (GNU) Bash as your shell, the commands here will be run each time you start a terminal (for example, when you open your terminal emulator in the graphic user interface). For security reasons, it is highly recommended to directly type in your ‘HOME’ directory value by hand in startup files instead of using variables. So in the following, let’s assume your user name is ‘‘name’’ (so ‘~’ may be replaced with ‘/home/name’). To add ‘~/.local/bin’ to your ‘PATH’ automatically on any startup file, you have to “export†the new value of ‘PATH’ in the startup file that is most relevant to you by adding this line: export PATH=$PATH:/home/name/.local/bin Now that you know your system will look into ‘~/.local/bin’ for executables, you can tell Gnuastro’s configure script to install everything in the top ‘~/.local’ directory using the ‘--prefix’ option. When you subsequently run ‘$ make install’, all the install-able files will be put in their respective directory under ‘~/.local/’ (the executables in ‘~/.local/bin’, the compiled library files in ‘~/.local/lib’, the library header files in ‘~/.local/include’ and so on, to learn more about these different files, please see *note Review of library fundamentals::). Note that tilde (‘<~>’) expansion will not happen if you put a ‘<=>’ between ‘--prefix’ and ‘~/.local’(3), so we have avoided the <=> character here which is optional in GNU-style options, see *note Options::. $ ./configure --prefix ~/.local You can install everything (including libraries like GSL, CFITSIO, or WCSLIB which are Gnuastro’s mandatory dependencies, see *note Mandatory dependencies::) locally by configuring them as above. However, recall that ‘PATH’ is only for executable files, not libraries and that libraries can also depend on other libraries. For example WCSLIB depends on CFITSIO and Gnuastro needs both. Therefore, when you installed a library in a non-recognized directory, you have to guide the program that depends on them to look into the necessary library and header file directories. To do that, you have to define the ‘LDFLAGS’ and ‘CPPFLAGS’ environment variables respectively. This can be done while calling ‘./configure’ as shown below: $ ./configure LDFLAGS=-L/home/name/.local/lib \ CPPFLAGS=-I/home/name/.local/include \ --prefix ~/.local It can be annoying/buggy to do this when configuring every software that depends on such libraries. Hence, you can define these two variables in the most relevant startup file (discussed above). The convention on using these variables doesn’t include a colon to separate values (as ‘PATH’-like variables do), they use white space characters and each value is prefixed with a compiler option(4): note the ‘-L’ and ‘-I’ above (see *note Options::), for ‘-I’ see *note Headers::, and for ‘-L’, see *note Linking::. Therefore we have to keep the value in double quotation signs to keep the white space characters and adding the following two lines to the startup file of choice: export LDFLAGS="$LDFLAGS -L/home/name/.local/lib" export CPPFLAGS="$CPPFLAGS -I/home/name/.local/include" Dynamic libraries are linked to the executable every time you run a program that depends on them (see *note Linking:: to fully understand this important concept). Hence dynamic libraries also require a special path variable called ‘LD_LIBRARY_PATH’ (same formatting as ‘PATH’). To use programs that depend on these libraries, you need to add ‘~/.local/lib’ to your ‘LD_LIBRARY_PATH’ environment variable by adding the following line to the relevant start-up file: export LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/home/name/.local/lib If you also want to access the Info (see *note Info::) and man pages (see *note Man pages::) documentations add ‘~/.local/share/info’ and ‘~/.local/share/man’ to your ‘INFOPATH’(5) and ‘MANPATH’ environment variables respectively. A final note is that order matters in the directories that are searched for all the variables discussed above. In the examples above, the new directory was added after the system specified directories. So if the program, library or manuals are found in the system wide directories, the user directory is no longer searched. If you want to search your local installation first, put the new directory before the already existing list, like the example below. export LD_LIBRARY_PATH=/home/name/.local/lib:$LD_LIBRARY_PATH This is good when a library, for example CFITSIO, is already present on the system, but the system-wide install wasn’t configured with the correct configuration flags (see *note CFITSIO::), or you want to use a newer version and you don’t have administrator or root access to update it on the whole system/server. If you update ‘LD_LIBRARY_PATH’ by placing ‘~/.local/lib’ first (like above), the linker will first find the CFITSIO you installed for yourself and link with it. It thus will never reach the system-wide installation. There are important security problems with using local installations first: all important system-wide executables and libraries (important executables like ‘ls’ and ‘cp’, or libraries like the C library) can be replaced by non-secure versions with the same file names and put in the customized directory (‘~/.local’ in this example). So if you choose to search in your customized directory first, please _be sure_ to keep it clean from executables or libraries with the same names as important system programs or libraries. *Summary:* When you are using a server which doesn’t give you administrator/root access AND you would like to give priority to your own built programs and libraries, not the version that is (possibly already) present on the server, add these lines to your startup file. See above for which startup file is best for your case and for a detailed explanation on each. Don’t forget to replace ‘‘/YOUR-HOME-DIR’’ with your home directory (for example ‘‘/home/your-id’’): export PATH="/YOUR-HOME-DIR/.local/bin:$PATH" export LDFLAGS="-L/YOUR-HOME-DIR/.local/lib $LDFLAGS" export MANPATH="/YOUR-HOME-DIR/.local/share/man/:$MANPATH" export CPPFLAGS="-I/YOUR-HOME-DIR/.local/include $CPPFLAGS" export INFOPATH="/YOUR-HOME-DIR/.local/share/info/:$INFOPATH" export LD_LIBRARY_PATH="/YOUR-HOME-DIR/.local/lib:$LD_LIBRARY_PATH" Afterwards, you just need to add an extra ‘--prefix=/YOUR-HOME-DIR/.local’ to the ‘./configure’ command of the software that you intend to install. Everything else will be the same as a standard build and install, see *note Quick start::. ---------- Footnotes ---------- (1) By running ‘$ export myvariable=a_test_value’ instead of the simpler case in the text (2) You can use shell variables for other actions too, for example to temporarily keep some names or run loops on some files. (3) If you insist on using ‘<=>’, you can use ‘--prefix=$HOME/.local’. (4) These variables are ultimately used as options while building the programs, so every value has be an option name followed be a value as discussed in *note Options::. (5) Info has the following convention: “If the value of ‘INFOPATH’ ends with a colon [or it isn’t defined] ..., the initial list of directories is constructed by appending the build-time default to the value of ‘INFOPATH’.†So when installing in a non-standard directory and if ‘INFOPATH’ was not initially defined, add a colon to the end of ‘INFOPATH’ as shown below, otherwise Info will not be able to find system-wide installed documentation: ‘echo 'export INFOPATH=$INFOPATH:/home/name/.local/share/info:' >> ~/.bashrc’ Note that this is only an internal convention of Info, do not use it for other ‘*PATH’ variables.  File: gnuastro.info, Node: Executable names, Next: Configure and build in RAM, Prev: Installation directory, Up: Configuring 3.3.1.3 Executable names ........................ At first sight, the names of the executables for each program might seem to be uncommonly long, for example ‘astnoisechisel’ or ‘astcrop’. We could have chosen terse (and cryptic) names like most programs do. We chose this complete naming convention (something like the commands in TeX) so you don’t have to spend too much time remembering what the name of a specific program was. Such complete names also enable you to easily search for the programs. To facilitate typing the names in, we suggest using the shell auto-complete. With this facility you can find the executable you want very easily. It is very similar to file name completion in the shell. For example, simply by typing the letters below (where <[TAB]> stands for the Tab key on your keyboard) $ ast[TAB][TAB] you will get the list of all the available executables that start with ‘ast’ in your ‘PATH’ environment variable directories. So, all the Gnuastro executables installed on your system will be listed. Typing the next letter for the specific program you want along with a Tab, will limit this list until you get to your desired program. In case all of this does not convince you and you still want to type short names, some suggestions are given below. You should have in mind though, that if you are writing a shell script that you might want to pass on to others, it is best to use the standard name because other users might not have adopted the same customizations. The long names also serve as a form of documentation in such scripts. A similar reasoning can be given for option names in scripts: it is good practice to always use the long formats of the options in shell scripts, see *note Options::. The simplest solution is making a symbolic link to the actual executable. For example let’s assume you want to type ‘ic’ to run Crop instead of ‘astcrop’. Assuming you installed Gnuastro executables in ‘/usr/local/bin’ (default) you can do this simply by running the following command as root: # ln -s /usr/local/bin/astcrop /usr/local/bin/ic In case you update Gnuastro and a new version of Crop is installed, the default executable name is the same, so your custom symbolic link still works. The installed executable names can also be set using options to ‘$ ./configure’, see *note Configuring::. GNU Autoconf (which configures Gnuastro for your particular system), allows the builder to change the name of programs with the three options ‘--program-prefix’, ‘--program-suffix’ and ‘--program-transform-name’. The first two are for adding a fixed prefix or suffix to all the programs that will be installed. This will actually make all the names longer! You can use it to add versions of program names to the programs in order to simultaneously have two executable versions of a program. The third configure option allows you to set the executable name at install time using the SED program. SED is a very useful ‘stream editor’. There are various resources on the internet to use it effectively. However, we should caution that using configure options will change the actual executable name of the installed program and on every re-install (an update for example), you have to also add this option to keep the old executable name updated. Also note that the documentation or configuration files do not change from their standard names either. For example, let’s assume that typing ‘ast’ on every invocation of every program is really annoying you! You can remove this prefix from all the executables at configure time by adding this option: $ ./configure --program-transform-name='s/ast/ /'  File: gnuastro.info, Node: Configure and build in RAM, Prev: Executable names, Up: Configuring 3.3.1.4 Configure and build in RAM .................................. The configure and build process involves the creation, reading, and modification of a large number of files (input/output, or I/O). Therefore file I/O issues can directly affect the work of developers who need to configure and build Gnuastro numerous times. Some of these issues are listed below: • I/O will cause wear and tear on both the HDDs (mechanical failures) and SSDs (decreasing the lifetime). • Having the built files mixed with the source files can greatly affect backing up (synchronization) of source files (since it involves the management of a large number of small files that are regularly changed. Backup software can of course be configured to ignore the built files and directories. However, since the built files are mixed with the source files and can have a large variety, this will require a high level of customization. One solution to address both these problems is to use the tmpfs file system (https://en.wikipedia.org/wiki/Tmpfs). Any file in tmpfs is actually stored in the RAM (and possibly SAWP), not on HDDs or SSDs. The RAM is built for extensive and fast I/O. Therefore the large number of file I/Os associated with configuring and building will not harm the HDDs or SSDs. Due to the volatile nature of RAM, files in the tmpfs file-system will be permanently lost after a power-off. Since all configured and built files are derivative files (not files that have been directly written by hand) there is no problem in this and this feature can be considered as an automatic cleanup. The modern GNU C library (and thus the Linux kernel) define the ‘/dev/shm’ directory for this purpose (POSIX shared memory). So using GNU Build System’s ability to build in a separate directory (not necessarily in the source directory), we can configure and build the programs in ‘/dev/shm’ to benefit from the RAM. To simplify the process, Gnuastro comes with a ‘tmpfs-config-make’ script. This script will create a directory in the shared memory, and put a symbolic link to it (called ‘build’) in the top source directory (the backup/sync software therefore only needs to ignore this single link/file). The script will then internally change to that directory and configure and build (‘make -kjN’, where ‘N’ is the number of threads for a parallel build) Gnuastro in there. To benefit from this script, simply run the following command instead of ‘./configure’ and ‘make’: $ ./tmpfs-config-make After this script is finished, you can ‘‘cd build’’ and run other Make commands (for example, ‘‘make check’’, ‘‘make install’’, or ‘‘make pdf’’) from there. In Emacs, the command to be run with the ‘M-x compile’ command (by default: ‘make -k’) can be changed to ‘‘cd build; make -kjN’’, or ‘‘make -C build -kjN’’ (‘N’ is the number of threads; an integer $\geq1$). For subsequent builds (during development) the ‘M-x recompile’ command will also do all the building in the RAM while you modify the clean, and backed-up source files and make minimal/efficient use of your non-volatile HDD or SSD. This script can be used in any software which is configured and built using the GNU Build System. Just copy it in the top source directory of that software and run it from there. The default number of threads and location of the shared memory (‘/dev/shm’) are currently hard-coded within the script. If you need to change them, please open the script with a text editor and set their values manually.  File: gnuastro.info, Node: Tests, Next: A4 print book, Prev: Configuring, Up: Build and install 3.3.2 Tests ----------- After successfully building (compiling) the programs with the ‘$ make’ command you can check the installation before installing. To run the tests, run $ make check For every program some tests are designed to check some possible operations. Running the command above will run those tests and give you a final report. If everything is ok and you have built all the programs, all the tests should pass. In case any of the tests fail, please have a look at *note Known issues:: and if that still doesn’t fix your problem, look that the ‘./tests/test-suite.log’ file to see if the source of the error is something particular to your system or more general. If you feel it is general, please contact us because it might be a bug. Note that the tests of some programs depend on the outputs of other program’s tests, so if you have not installed them they might be skipped or fail. Prior to releasing every distribution all these tests are checked. If you have a reasonably modern terminal, the outputs of the successful tests will be colored green and the failed ones will be colored red. These scripts can also act as a good set of examples for you to see how the programs are run. All the tests are in the ‘tests/’ directory. The tests for each program are shell scripts (ending with ‘.sh’) in a sub-directory of this directory with the same name as the program. See *note Test scripts:: for more detailed information about these scripts in case you want to inspect them.  File: gnuastro.info, Node: A4 print book, Next: Known issues, Prev: Tests, Up: Build and install 3.3.3 A4 print book ------------------- The default print version of this book is provided in the letter paper size. If you would like to have the print version of this book on paper and you are living in a country which uses A4, then you can rebuild the book. The great thing about the GNU build system is that the book source code which is in Texinfo is also distributed with the program source code, enabling you to do such customizations (hacking). In order to change the paper size, you will need to have GNU Texinfo installed. Open ‘doc/gnuastro.texi’ with any text editor. This is the source file that created this book. In the first few lines you will see this line: @c@afourpaper In Texinfo, a line is commented with ‘@c’. Therefore, un-comment this line by deleting the first two characters such that it changes to: @afourpaper Save the file and close it. You can now run $ make pdf and the new PDF book will be available in ‘SRCdir/doc/gnuastro.pdf’. By changing the ‘pdf’ in ‘$ make pdf’ to ‘ps’ or ‘dvi’ you can have the book in those formats. Note that you can do this for any book that is in Texinfo format, they might not have ‘@afourpaper’ line, so you can add it close to the top of the Texinfo source file.  File: gnuastro.info, Node: Known issues, Prev: A4 print book, Up: Build and install 3.3.4 Known issues ------------------ Depending on your operating system and the version of the compiler you are using, you might confront some known problems during the configuration (‘$ ./configure’), compilation (‘$ make’) and tests (‘$ make check’). Here, their solutions are discussed. • ‘$ ./configure’: _Configure complains about not finding a library even though you have installed it._ The possible solution is based on how you installed the package: • From your distribution’s package manager. Most probably this is because your distribution has separated the header files of a library from the library parts. Please also install the ‘development’ packages for those libraries too. Just add a ‘-dev’ or ‘-devel’ to the end of the package name and re-run the package manager. This will not happen if you install the libraries from source. When installed from source, the headers are also installed. • From source. Then your linker is not looking where you installed the library. If you followed the instructions in this chapter, all the libraries will be installed in ‘/usr/local/lib’. So you have to tell your linker to look in this directory. To do so, add ‘LDFLAGS=-L/usr/local/lib’ to the Gnuastro configure script. If you want to use the libraries for your other programming projects, then export this environment variable similar to the case for ‘LD_LIBRARY_PATH’ explained below. • ‘$ make’: _Complains about an unknown function on a non-GNU based operating system._ In this case, please run ‘$ ./configure’ with the ‘--enable-gnulibcheck’ option to see if the problem is from the GNU Portability Library (Gnulib) not supporting your system or if there is a problem in Gnuastro, see *note Gnuastro configure options::. If the problem is not in Gnulib and after all its tests you get the same complaint from ‘make’, then please contact us at ‘bug-gnuastro@gnu.org’. The cause is probably that a function that we have used is not supported by your operating system and we didn’t included it along with the source tar ball. If the function is available in Gnulib, it can be fixed immediately. • ‘$ make’: _Can’t find the headers (.h files) of libraries installed from source._ Similar to the case for ‘LDFLAGS’ (above), your compiler is not looking in the right place, add ‘CPPFLAGS=-I/usr/local/include’ to ‘./configure’ to re-configure Gnuastro, then re-run make. • ‘$ make check’: _Only one ‘.sh’ test passes, all the rest fail._ It is highly likely that your distribution doesn’t look into the ‘/usr/local/lib’ directory when searching for shared libraries. To make sure it is added to the list of directories, run the following command and restart your terminal: (you can ignore the ‘\’ and extra space if you type it, it is only necessary if you copy and paste). See *note Installation directory:: for more details. echo 'export LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/lib' \ >> ~/.bashrc • ‘$ make check’: _The tests relying on external programs (for example ‘fitstopdf.sh’ fail._) This is probably due to the fact that the version number of the external programs is too old for the tests we have preformed. Please update the program to a more recent version. For example to create a PDF image, you will need GPL Ghostscript, but older versions do not work, we have successfully tested it on version 9.15. Older versions might cause a failure in the test result. • ‘$ make pdf’: _The PDF book cannot be made._ To make a PDF book, you need to have the GNU Texinfo program (like any program, the more recent the better). A working TeX program is also necessary, which you can get from Tex Live(1). • After ‘make check’: do not copy the programs’ executables to another (for example, the installation) directory manually (using ‘cp’, or ‘mv’ for example). In the default configuration(2), the program binaries need to link with Gnuastro’s shared library which is also built and installed with the programs. Therefore, to run successfully before and after installation, linking modifications need to be made by GNU Libtool at installation time. ‘make install’ does this internally, but a simple copy might give linking errors when you run it. If you need to copy the executables, you can do so after installation. If your problem was not listed above, please file a bug report (*note Report a bug::). ---------- Footnotes ---------- (1) (2) If you configure Gnuastro with the ‘--disable-shared’ option, then the libraries will be statically linked to the programs and this problem won’t exist, see *note Linking::.  File: gnuastro.info, Node: Common program behavior, Next: Data containers, Prev: Installation, Up: Top 4 Common program behavior ************************* All the programs in Gnuastro share a set of common behavior mainly to do with user interaction to facilitate their usage. The most basic is how you can configure each program to do what you want: define the input, change parameter/option values, or identify the output. All Gnuastro programs can also read your desired configuration from pre-defined or user-specified files so you don’t have to specify all the (sometimes numerous) parameters on the command-line each time you run a program. These files define the “default†program behavior in each directory, for each user, or on each system. In other cases, some programs can greatly benefit from the many threads available in modern CPUs, so here we’ll also discuss how you can get the most out of your hardware. Among some other issues, we will also discuss how you can get immediate and distraction-free (without taking your hands off the keyboard!) help, or access to this whole book, on the command-line. * Menu: * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Multi-threaded operations:: How threads are managed in Gnuastro. * Numeric data types:: Different types and how to specify them. * Tables:: Recognized table formats. * Tessellation:: Tile the dataset into non-overlapping bins. * Getting help:: Getting more information on the go. * Automatic output:: About automatic output names. * Output headers:: Common headers to all FITS outputs.  File: gnuastro.info, Node: Command-line, Next: Configuration files, Prev: Common program behavior, Up: Common program behavior 4.1 Command-line ================ All the programs in Gnuastro are customized through the standard GNU style command-line options. Thus, we’ll start by defining this general style that is very common in many command-line tools on Unix-like operating systems. Finally, the options that are common to all the programs in Gnuastro are discussed. The command-line text that you type is passed onto the shell (or program managing the command-line) as a string of characters. See the “Invoking ProgramName†sections in this manual for some examples of commands with each program, for example *note Invoking asttable::. That string is then broken up into separate _tokens_ or _words_ by any _metacharacters_ (like space, tab, ‘|’, ‘>’ or ‘;’) that might exist in the text. To learn more, please see the GNU Bash manual, for the complete list of meta-characters and other GNU Bash definitions (GNU Bash is the most common shell program). Its “Shell Operation†section has a short summary of the steps the shell takes before passing the commands to the program you called. * Menu: * Arguments and options:: Basics of options and arguments. * Common options:: Common options to all Gnuastro programs.  File: gnuastro.info, Node: Arguments and options, Next: Common options, Prev: Command-line, Up: Command-line 4.1.1 Arguments and options --------------------------- On the command-line, the first thing you usually enter is the name of the program you want to run. After that, you can specify two types of input: _arguments_ and _options_. In the GNU-style, arguments are those tokens that are not preceded by any hyphens (‘-’, see *note Arguments::). Here is one example: $ astcrop --center=53.162551,-27.789676 -w10/3600 --mode=wcs udf.fits In this example, the argument is ‘udf.fits’. Arguments are most commonly the input file names containing your data. Options start with one or two hyphens, followed by an identifier for the option (the option’s name) and its value (see *note Options::). Through options you tell the program how to interpret the data. In this example, we are running *note Crop:: to crop a region of width 10 arc-seconds centered at the given RA and Dec from the input Hubble Ultra-Deep Field (UDF) FITS image. So options come with an identifier (the option name which is separate from their value). Arguments can be both mandatory and optional and unlike options they don’t have any identifiers (or help from you). Hence, their order might also matter (for example in ‘cp’ which is used for copying one file to another location). The outputs of ‘--usage’ and ‘--help’ shows which arguments are optional and which are mandatory, see *note --usage::. As their name suggests, _options_ on the command-line can be considered to be optional and most of the time, you don’t have to worry about what order you specify them in. When the order does matter, or the option can be invoked multiple times, it is explicitly mentioned in the “Invoking ProgramName†section of each program. In case your arguments or option values contain any of the shell’s meta-characters, you have to quote them. If there is only one such character, you can use a backslash (‘\’) before it. If there are multiple, it might be easier to simply put your whole argument or option value inside of double quotes (‘"’). In such cases, everything inside the double quotes will be seen as one token or word. For example, let’s say you want to specify the header data unit (HDU) of your FITS file using a complex expression like ‘‘3; images(exposure > 100)’’. If you simply add these after the ‘--hdu’ (‘-h’) option, the programs in Gnuastro will read the value to the HDU option as ‘‘3’’ and run. Then, Bash will attempt to run a separate command ‘‘images(exposure > 100)’’ and complain about a syntax error. This is because the semicolon (‘;’) is an ‘end of command’ character in the shell. To solve this problem you can simply put double quotes around the whole string you want to pass to ‘--hdu’ as seen below: $ astcrop --hdu="3; images(exposure > 100)" FITSimage.fits Alternatively you can put a ‘‘\’’ before every meta-character in this string, but try doing that, and probably you will agree that the double quotes are much more easier, elegant and readable. * Menu: * Arguments:: For specifying the main input files/operations. * Options:: For configuring the behavior of the program.  File: gnuastro.info, Node: Arguments, Next: Options, Prev: Arguments and options, Up: Arguments and options 4.1.1.1 Arguments ................. In Gnuastro, arguments are almost exclusively used as the input data file names. Please consult the first few paragraph of the “Invoking ProgramName†section for each program for a description of what it expects as input, how many arguments, or input data, it accepts, or in what order. Everything particular about how a program treats arguments, is explained under the “Invoking ProgramName†section for that program. Generally, if there is a standard file name extension for a particular format, that filename extension is used to separate the kinds of arguments. The list below shows the data formats that are recognized in Gnuastro’s programs based on their file name endings. Any argument that doesn’t end with the specified extensions below is considered to be a text file (usually catalogs, see *note Tables::). In some cases, a program can accept specific formats, for example *note ConvertType:: also accepts ‘.jpg’ images. • ‘.fits’: The standard file name ending of a FITS image. • ‘.fit’: Alternative (3 character) FITS suffix. • ‘.fits.Z’: A FITS image compressed with ‘compress’. • ‘.fits.gz’: A FITS image compressed with GNU zip (gzip). • ‘.fits.fz’: A FITS image compressed with ‘fpack’. • ‘.imh’: IRAF format image file. Through out this book and in the command-line outputs, whenever we want to generalize all such astronomical data formats in a text place holder, we will use ‘ASTRdata’, we will assume that the extension is also part of this name. Any file ending with these names is directly passed on to CFITSIO to read. Therefore you don’t necessarily have to have these files on your computer, they can also be located on an FTP or HTTP server too, see the CFITSIO manual for more information. CFITSIO has its own error reporting techniques, if your input file(s) cannot be opened, or read, those errors will be printed prior to the final error by Gnuastro.  File: gnuastro.info, Node: Options, Prev: Arguments, Up: Arguments and options 4.1.1.2 Options ............... Command-line options allow configuring the behavior of a program in all GNU/Linux applications for each particular execution on a particular input data. A single option can be called in two ways: _long_ or _short_. All options in Gnuastro accept the long format which has two hyphens an can have many characters (for example ‘--hdu’). Short options only have one hyphen (<->) followed by one character (for example ‘-h’). You can see some examples in the list of options in *note Common options:: or those for each program’s “Invoking ProgramName†section. Both formats are shown for those which support both. First the short is shown then the long. Usually, the short options are for when you are writing on the command-line and want to save keystrokes and time. The long options are good for shell scripts, where you aren’t usually rushing. Long options provide a level of documentation, since they are more descriptive and less cryptic. Usually after a few months of not running a program, the short options will be forgotten and reading your previously written script will not be easy. Some options need to be given a value if they are called and some don’t. You can think of the latter type of options as on/off options. These two types of options can be distinguished using the output of the ‘--help’ and ‘--usage’ options, which are common to all GNU software, see *note Getting help::. In Gnuastro we use the following strings to specify when the option needs a value and what format that value should be in. More specific tests will be done in the program and if the values are out of range (for example negative when the program only wants a positive value), an error will be reported. ‘INT’ The value is read as an integer. ‘FLT’ The value is read as a float. There are generally two types, depending on the context. If they are for fractions, they will have to be less than or equal to unity. ‘STR’ The value is read as a string of characters (for example a file name) or other particular settings like a HDU name, see below. To specify a value in the short format, simply put the value after the option. Note that since the short options are only one character long, you don’t have to type anything between the option and its value. For the long option you either need white space or an ‘=’ sign, for example ‘-h2’, ‘-h 2’, ‘--hdu 2’ or ‘--hdu=2’ are all equivalent. The short format of on/off options (those that don’t need values) can be concatenated for example these two hypothetical sequences of options are equivalent: ‘-a -b -c4’ and ‘-abc4’. As an example, consider the following command to run Crop: $ astcrop -Dr3 --wwidth 3 catalog.txt --deccol=4 ASTRdata The ‘$’ is the shell prompt, ‘astcrop’ is the program name. There are two arguments (‘catalog.txt’ and ‘ASTRdata’) and four options, two of them given in short format (‘-D’, ‘-r’) and two in long format (‘--width’ and ‘--deccol’). Three of them require a value and one (‘-D’) is an on/off option. If an abbreviation is unique between all the options of a program, the long option names can be abbreviated. For example, instead of typing ‘--printparams’, typing ‘--print’ or maybe even ‘--pri’ will be enough, if there are conflicts, the program will warn you and show you the alternatives. Finally, if you want the argument parser to stop parsing arguments beyond a certain point, you can use two dashes: ‘--’. No text on the command-line beyond these two dashes will be parsed. Gnuastro has two types of options with values, those that only take a single value are the most common type. If these options are repeated or called more than once on the command-line, the value of the last time it was called will be assigned to it. This is very useful when you are testing/experimenting. Let’s say you want to make a small modification to one option value. You can simply type the option with a new value in the end of the command and see how the script works. If you are satisfied with the change, you can remove the original option for human readability. If the change wasn’t satisfactory, you can remove the one you just added and not worry about forgetting the original value. Without this capability, you would have to memorize or save the original value somewhere else, run the command and then change the value again which is not at all convenient and is potentially cause lots of bugs. On the other hand, some options can be called multiple times in one run of a program and can thus take multiple values (for example see the ‘--column’ option in *note Invoking asttable::. In these cases, the order of stored values is the same order that you specified on the command-line. Gnuastro’s programs don’t keep any internal default values, so some options are mandatory and if they don’t have a value, the program will complain and abort. Most programs have many such options and typing them by hand on every call is impractical. To facilitate the user experience, after parsing the command-line, Gnuastro’s programs read special configuration files to get the necessary values for the options you haven’t identified on the command-line. These configuration files are fully described in *note Configuration files::. *CAUTION:* In specifying a file address, if you want to use the shell’s tilde expansion (‘~’) to specify your home directory, leave at least one space between the option name and your value. For example use ‘-o ~/test’, ‘--output ~/test’ or ‘--output= ~/test’. Calling them with ‘-o~/test’ or ‘--output=~/test’ will disable shell expansion. *CAUTION:* If you forget to specify a value for an option which requires one, and that option is the last one, Gnuastro will warn you. But if it is in the middle of the command, it will take the text of the next option or argument as the value which can cause undefined behavior. *NOTE:* In some contexts Gnuastro’s counting starts from 0 and in others 1. You can assume by default that counting starts from 1, if it starts from 0 for a special option, it will be explicitly mentioned.  File: gnuastro.info, Node: Common options, Prev: Arguments and options, Up: Command-line 4.1.2 Common options -------------------- To facilitate the job of the users and developers, all the programs in Gnuastro share some basic command-line options for the options that are common to many of the programs. The full list is classified as *note Input output options::, *note Processing options::, and *note Operating mode options::. In some programs, some of the options are irrelevant, but still recognized (you won’t get an unrecognized option error, but the value isn’t used). Unless otherwise mentioned, these options are identical between all programs. * Menu: * Input output options:: Common input/output options. * Processing options:: Options for common processing steps. * Operating mode options:: Common operating mode options.  File: gnuastro.info, Node: Input output options, Next: Processing options, Prev: Common options, Up: Common options 4.1.2.1 Input/Output options ............................ These options are to do with the input and outputs of the various programs. ‘-h STR/INT’ ‘--hdu=STR/INT’ The name or number of the desired Header Data Unit, or HDU, in the FITS image. A FITS file can store multiple HDUs or extensions, each with either an image or a table or nothing at all (only a header). Note that counting of the extensions starts from 0(zero), not 1(one). Counting from 0 is forced on us by CFITSIO which directly reads the value you give with this option (see *note CFITSIO::). When specifying the name, case is not important so ‘IMAGE’, ‘image’ or ‘ImAgE’ are equivalent. CFITSIO has many capabilities to help you find the extension you want, far beyond the simple extension number and name. See CFITSIO manual’s “HDU Location Specification†section for a very complete explanation with several examples. A ‘#’ is appended to the string you specify for the HDU(1) and the result is put in square brackets and appended to the FITS file name before calling CFITSIO to read the contents of the HDU for all the programs in Gnuastro. ‘-s STR’ ‘--searchin=STR’ Where to match/search for columns when the column identifier wasn’t a number, see *note Selecting table columns::. The acceptable values are ‘name’, ‘unit’, or ‘comment’. This option is only relevant for programs that take table columns as input. ‘-I’ ‘--ignorecase’ Ignore case while matching/searching column meta-data (in the field specified by the ‘--searchin’). The FITS standard suggests to treat the column names as case insensitive, which is strongly recommended here also but is not enforced. This option is only relevant for programs that take table columns as input. This option is not relevant to *note BuildProgram::, hence in that program the short option ‘-I’ is used for include directories, not to ignore case. ‘-o STR’ ‘--output=STR’ The name of the output file or directory. With this option the automatic output names explained in *note Automatic output:: are ignored. ‘-T STR’ ‘--type=STR’ The data type of the output depending on the program context. This option isn’t applicable to some programs like *note Fits:: and will be ignored by them. The different acceptable values to this option are fully described in *note Numeric data types::. ‘-D’ ‘--dontdelete’ By default, if the output file already exists, Gnuastro’s programs will silently delete it and put their own outputs in its place. When this option is activated, if the output file already exists, the programs will not delete it, will warn you, and will abort. ‘-K’ ‘--keepinputdir’ In automatic output names, don’t remove the directory information of the input file names. As explained in *note Automatic output::, if no output name is specified (with ‘--output’), then the output name will be made in the existing directory based on your input’s file name (ignoring the directory of the input). If you call this option, the directory information of the input will be kept and the automatically generated output name will be in the same directory as the input (usually with a suffix added). Note that his is only relevant if you are running the program in a different directory than the input data. ‘-t STR’ ‘--tableformat=STR’ The output table’s type. This option is only relevant when the output is a table and its format cannot be deduced from its filename. For example, if a name ending in ‘.fits’ was given to ‘--output’, then the program knows you want a FITS table. But there are two types of FITS tables: FITS ASCII, and FITS binary. Thus, with this option, the program is able to identify which type you want. The currently recognized values to this option are: ‘txt’ A plain text table with white-space characters between the columns (see *note Gnuastro text table format::). ‘fits-ascii’ A FITS ASCII table (see *note Recognized table formats::). ‘fits-binary’ A FITS binary table (see *note Recognized table formats::). ---------- Footnotes ---------- (1) With the ‘#’ character, CFITSIO will only read the desired HDU into your memory, not all the existing HDUs in the fits file.  File: gnuastro.info, Node: Processing options, Next: Operating mode options, Prev: Input output options, Up: Common options 4.1.2.2 Processing options .......................... Some processing steps are common to several programs, so they are defined as common options to all programs. Note that this class of common options is thus necessarily less common between all the programs than those described in *note Input output options::, or *note Operating mode options:: options. Also, if they are irrelevant for a program, these options will not display in the ‘--help’ output of the program. ‘--minmapsize=INT’ The minimum size (in bytes) to store the contents of each main processing array of a program as a file (on the non-volatile HDD/SSD), not in RAM. This can be very useful for large datasets which can be very memory intensive such that your RAM will not be sufficient to keep/process them. A random filename is assigned to the array (in a ‘.gnuastro’ directory within the running directory) which will keep the contents of the array as long as it is necessary. When this option has a value of ‘0’ (zero), all arrays that use this option in a program will actually be in a file (not in RAM). When the value is ‘-1’ (largest possible number in the unsigned integer types) these arrays will be definitely allocated in RAM. However, for complex programs like *note NoiseChisel::, it is recommended to not set it to ‘0’, but a value like ‘10000’ so the many small arrays necessary during processing are stored in RAM and only larger ones are saved as a file. Please note that using a non-volatile file (in the HDD/SDD) instead of RAM can significantly increase the program’s running time, especially on HDDs. So it is best to give this option large values by default. You can then decrease it for a specific program’s invocation on a large input after you see memory issues arise (for example an error, or the program not aborting and fully consuming your memory). The random file will be deleted once it is no longer needed by the program. The ‘.gnuastro’ directory will also be deleted if it has no other contents (you may also have configuration files in this directory, see *note Configuration files::). If you see randomly named files remaining in this directory, please send us a bug report so we address the problem, see *note Report a bug::. ‘-Z INT[,INT[,...]]’ ‘--tilesize=[,INT[,...]]’ The size of regular tiles for tessellation, see *note Tessellation::. For each dimension an integer length (in units of data-elements or pixels) is necessary. If the number of input dimensions is different from the number of values given to this option, the program will stop with an error. Values must be separated by commas (<,>) and can also be fractions (for example ‘4/2’). If they are fractions, the result must be an integer, otherwise an error will be printed. ‘-M INT[,INT[,...]]’ ‘--numchannels=INT[,INT[,...]]’ The number of channels for larger input tessellation, see *note Tessellation::. The number and types of acceptable values are similar to ‘--tilesize’. The only difference is that instead of length, the integers values given to this option represent the _number_ of channels, not their size. ‘-F FLT’ ‘--remainderfrac=FLT’ The fraction of remainder size along all dimensions to add to the first tile. See *note Tessellation:: for a complete description. This option is only relevant if ‘--tilesize’ is not exactly divisible by the input dataset’s size in a dimension. If the remainder size is larger than this fraction (compared to ‘--tilesize’), then the remainder size will be added with one regular tile size and divided between two tiles at the start and end of the given dimension. ‘--workoverch’ Ignore the channel borders for the high-level job of the given application. As a result, while the channel borders are respected in defining the small tiles (such that no tile will cross a channel border), the higher-level program operation will ignore them, see *note Tessellation::. ‘--checktiles’ Make a FITS file with the same dimensions as the input but each pixel is replaced with the ID of the tile that it is associated with. Note that the tile IDs start from 0. See *note Tessellation:: for more on Tiling an image in Gnuastro. ‘--oneelempertile’ When showing the tile values (for example with ‘--checktiles’, or when the program’s output is tessellated) only use one element for each tile. This can be useful when only the relative values given to each tile compared to the rest are important or need to be checked. Since the tiles usually have a large number of pixels within them the output will be much smaller, and so easier to read, write, store, or send. Note that when the full input size in any dimension is not exactly divisible by the given ‘--tilesize’ in that dimension, the edge tile(s) will have different sizes (in units of the input’s size), see ‘--remainderfrac’. But with this option, all displayed values are going to have the (same) size of one data-element. Hence, in such cases, the image proportions are going to be slightly different with this option. If your input image is not exactly divisible by the tile size and you want one value per tile for some higher-level processing, all is not lost though. You can see how many pixels were within each tile (for example to weight the values or discard some for later processing) with Gnuastro’s Statistics (see *note Statistics::) as shown below. The output FITS file is going to have two extensions, one with the median calculated on each tile and one with the number of elements that each tile covers. You can then use the ‘where’ operator in *note Arithmetic:: to set the values of all tiles that don’t have the regular area to a blank value. $ aststatistics --median --number --ontile input.fits \ --oneelempertile --output=o.fits $ REGULAR_AREA=1600 # Check second extension of `o.fits'. $ astarithmetic o.fits o.fits $REGULAR_AREA ne nan where \ -h1 -h2 Note that if ‘input.fits’ also has blank values, then the median on tiles with blank values will also be ignored with the command above (which is desirable). ‘--inteponlyblank’ When values are to be interpolated, only change the values of the blank elements, keep the non-blank elements untouched. ‘--interpnumngb=INT’ The number of nearby non-blank neighbors to use for interpolation.  File: gnuastro.info, Node: Operating mode options, Prev: Processing options, Up: Common options 4.1.2.3 Operating mode options .............................. Another group of options that are common to all the programs in Gnuastro are those to do with the general operation of the programs. The explanation for those that are not only limited to Gnuastro but are common to all GNU programs start with (GNU option). ‘--’ (GNU option) Stop parsing the command-line. This option can be useful in scripts or when using the shell history. Suppose you have a long list of options, and want to see if removing some of them (to read from configuration files, see *note Configuration files::) can give a better result. If the ones you want to remove are the last ones on the command-line, you don’t have to delete them, you can just add ‘--’ before them and if you don’t get what you want, you can remove the ‘--’ and get the same initial result. ‘--usage’ (GNU option) Only print the options and arguments and abort. This is very useful for when you know the what the options do, and have just forgot their long/short identifiers, see *note --usage::. ‘-?’ ‘--help’ (GNU option) Print all options with an explanation and abort. Adding this option will print all the options in their short and long formats, also displaying which ones need a value if they are called (with an ‘=’ after the long format followed by a string specifying the format, see *note Options::). A short explanation is also given for what the option is for. The program will quit immediately after the message is printed and will not do any form of processing, see *note --help::. ‘-V’ ‘--version’ (GNU option) Print a short message, showing the full name, version, copyright information and program authors and abort. On the first line, it will print the official name (not executable name) and version number of the program. Following this is a blank line and a copyright information. The program will not run. ‘-q’ ‘--quiet’ Don’t report steps. All the programs in Gnuastro that have multiple major steps will report their steps for you to follow while they are operating. If you do not want to see these reports, you can call this option and only error/warning messages will be printed. If the steps are done very fast (depending on the properties of your input) disabling these reports will also decrease running time. ‘--cite’ Print the BibTeX entry for Gnuastro and the particular program (if that program comes with a separate paper) and abort. Citations are vital for the continued work on Gnuastro. Gnuastro started and is continued based on separate research projects. So if you find any of the tools offered in Gnuastro to be useful in your research, please use the output of this command to cite the program and Gnuastro in your research paper. Thank you. Gnuastro is still new, there is no separate paper only devoted to Gnuastro yet. Therefore currently the paper to cite for Gnuastro is the paper for NoiseChisel which is the first published paper introducing Gnuastro to the astronomical community. Upon reaching a certain point, a paper completely devoted to Gnuastro will be published, see *note GNU Astronomy Utilities 1.0::. ‘-P’ ‘--printparams’ With this option, Gnuastro’s programs will read your command-line options and all the configuration files. If there is no problem (like a missing parameter or a value in the wrong format or range) and immediately before actually running, the programs will print the full list of option names, values and descriptions, sorted and grouped by context and abort. They will also report the version number, the date they were configured on your system and the time they were reported. As an example, you can give your full command-line options and even the input and output file names and finally just add ‘-P’ to check if all the parameters are finely set. If everything is ok, you can just run the same command (easily retrieved from the shell history, with the top arrow key) and simply remove the last two characters that showed this option. Since no program will actually start its processing when this option is called, the otherwise mandatory arguments for each program (for example input image or catalog files) are no longer required when you call this option. ‘--config=STR’ Parse ‘STR’ as a configuration file immediately when this option is confronted (see *note Configuration files::). The ‘--config’ option can be called multiple times in one run of any Gnuastro program on the command-line or in the configuration files. In any case, it will be immediately read (before parsing the rest of the options on the command-line, or lines in a configuration file). Note that by definition, later options on the command-line still take precedence over those in these in any configuration file, including the file(s) given to this option. Also see ‘--lastconfig’ and ‘--onlyversion’ on how this option can be used for reproducible results. ‘-S’ ‘--setdirconf’ Update the current directory configuration file for the Gnuastro program and quit. The full set of command-line and configuration file options will be parsed and options with a value will be written in the current directory configuration file for this program (see *note Configuration files::). If the configuration file or its directory doesn’t exist, it will be created. If a configuration file exists it will be replaced (after it, and all other configuration files have been read). In any case, the program will not run. This is the recommended method(1) to edit/set the configuration file for all future calls to Gnuastro’s programs. It will internally check if your values are in the correct range and type and save them according to the configuration file format, see *note Configuration file format::. So if there are unreasonable values to some options, the program will notify you and abort before writing the final configuration file. When this option is called, the otherwise mandatory arguments, for example input image or catalog file(s), are no longer mandatory (since the program will not run). ‘-U’ ‘--setusrconf’ Update the user configuration file and quit (see *note Configuration files::). See explanation under ‘--setdirconf’ for more details. ‘--lastconfig’ This is the last configuration file that must be read. When this option is confronted in any stage of reading the options (on the command-line or in a configuration file), no other configuration file will be parsed, see *note Configuration file precedence:: and *note Current directory and User wide::. Like all on/off options, on the command-line, this option doesn’t take any values. But in a configuration file, it takes the values of ‘0’ or ‘1’, see *note Configuration file format::. If it is present in a configuration file with a value of ‘0’, then all later occurrences of this option will be ignored. ‘--onlyversion=STR’ Only run the program if Gnuastro’s version is exactly equal to ‘STR’ (see *note Version numbering::). Note that it is not compared as a number, but as a string of characters, so ‘0’, or ‘0.0’ and ‘0.00’ are different. If the running Gnuastro version is different, then this option will report an error and abort as soon as it is confronted on the command-line or in a configuration file. If the running Gnuastro version is the same as ‘STR’, then the program will run as if this option was not called. This is useful if you want your results to be exactly reproducible and not mistakenly run with an updated/newer or older version of the program. Besides internal algorithmic/behavior changes in programs, the existence of options or their names might change between versions (especially in these earlier versions of Gnuastro). Hence, when using this option (probably in a script or in a configuration file), be sure to call it before other options. The benefit is that, when the version differs, the other options won’t be parsed and you, or your collaborators/users, won’t get errors saying an option in your configuration doesn’t exist in the running version of the program. Here is one example of how this option can be used in conjunction with the ‘--lastconfig’ option. Let’s assume that you were satisfied with the results of this command: ‘astnoisechisel image.fits --detquant=0.95’ (along with various options set in various configuration files). You can save the state of NoiseChisel and reproduce that exact result on ‘image.fits’ later by following these steps (the the extra spaces, and <\>, are only for easy readability, if you want to try it out, only one space between each token is enough). $ echo "onlyversion X.XX" > reproducible.conf $ echo "lastconfig 1" >> reproducible.conf $ astnoisechisel image.fits --detquant=0.95 -P \ >> reproducible.conf ‘--onlyversion’ was available from Gnuastro 0.0, so putting it immediately at the start of a configuration file will ensure that later, you (or others using different version) won’t get a non-recognized option error in case an option was added/removed. ‘--lastconfig’ will inform the installed NoiseChisel to not parse any other configuration files. This is done because we don’t want the user’s user-wide or system wide option values affecting our results. Finally, with the third command, which has a ‘-P’ (short for ‘--printparams’), NoiseChisel will print all the option values visible to it (in all the configuration files) and the shell will append them to ‘reproduce.conf’. Hence, you don’t have to worry about remembering the (possibly) different options in the different configuration files. Afterwards, if you run NoiseChisel as shown below (telling it to read this configuration file with the ‘--config’ option). You can be sure that there will either be an error (for version mis-match) or it will produce exactly the same result that you got before. $ astnoisechisel --config=reproducible.conf ‘--log’ Some programs can generate extra information about their outputs in a log file. When this option is called in those programs, the log file will also be printed. If the program doesn’t generate a log file, this option is ignored. ‘-N INT’ ‘--numthreads=INT’ Use ‘INT’ CPU threads when running a Gnuastro program (see *note Multi-threaded operations::). If the value is zero (‘0’), or this option is not given on the command-line or any configuration file, the value will be determined at run-time: the maximum number of threads available to the system when you run a Gnuastro program. Note that multi-threaded programming is only relevant to some programs. In others, this option will be ignored. ---------- Footnotes ---------- (1) Alternatively, you can use your favorite text editor.  File: gnuastro.info, Node: Configuration files, Next: Multi-threaded operations, Prev: Command-line, Up: Common program behavior 4.2 Configuration files ======================= Each program needs a certain number of parameters to run. Supplying all the necessary parameters each time you run the program is very frustrating and prone to errors. Therefore all the programs read the values for the necessary options you have not given in the command line from one of several plain text files (which you can view and edit with any text editor). These files are known as configuration files and are usually kept in a directory named ‘etc/’ according to the file system hierarchy standard(1). The thing to have in mind is that none of the programs in Gnuastro keep any internal default value. All the values must either be stored in one of the configuration files or explicitly called in the command-line. In case the necessary parameters are not given through any of these methods, the program will print a missing option error and abort. The only exception to this is ‘--numthreads’, whose default value is determined at run-time using the number of threads available to your system, see *note Multi-threaded operations::. Of course, you can still provide a default value for the number of threads at any of the levels below, but if you don’t, the program will not abort. Also note that through automatic output name generation, the value to the ‘--output’ option is also not mandatory on the command-line or in the configuration files for all programs which don’t rely on that value as an input(2), see *note Automatic output::. * Menu: * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. ---------- Footnotes ---------- (1) (2) One example of a program which uses the value given to ‘--output’ as an input is ConvertType, this value specifies the type of the output through the value to ‘--output’, see *note Invoking astconvertt::.  File: gnuastro.info, Node: Configuration file format, Next: Configuration file precedence, Prev: Configuration files, Up: Configuration files 4.2.1 Configuration file format ------------------------------- The configuration files for each program have the standard program executable name with a ‘‘.conf’’ suffix. When you download the source code, you can find them in the same directory as the source code of each program, see *note Program source::. Any line in the configuration file whose first non-white character is a <#> is considered to be a comment and is ignored. An empty line is also similarly ignored. The long name of the option should be used as an identifier. The parameter name and parameter value have to be separated by any number of ‘white-space’ characters: space, tab or vertical tab. By default several space characters are used. If the value of an option has space characters (most commonly for the ‘hdu’ option), then the full value can be enclosed in double quotation signs (<">, similar to the example in *note Arguments and options::). If it is an option without a value in the ‘--help’ output (on/off option, see *note Options::), then the value should be ‘1’ if it is to be ‘on’ and ‘0’ otherwise. In each non-commented and non-blank line, any text after the first two words (option identifier and value) is ignored. If an option identifier is not recognized in the configuration file, the name of the file, the line number of the unrecognized option, and the unrecognized identifier name will be reported and the program will abort. If a parameter is repeated more more than once in the configuration files, accepts only one value, and is not set on the command-line, then only the first value will be used, the rest will be ignored. You can build or edit any of the directories and the configuration files yourself using any text editor. However, it is recommended to use the ‘--setdirconf’ and ‘--setusrconf’ options to set default values for the current directory or this user, see *note Operating mode options::. With these options, the values you give will be checked before writing in the configuration file. They will also print a set of commented lines guiding the reader and will also classify the options based on their context and write them in their logical order to be more understandable.  File: gnuastro.info, Node: Configuration file precedence, Next: Current directory and User wide, Prev: Configuration file format, Up: Configuration files 4.2.2 Configuration file precedence ----------------------------------- The option values in all the programs of Gnuastro will be filled in the following order. If an option only takes one value which is given in an earlier step, any value for that option in a later step will be ignored. Note that if the ‘lastconfig’ option is specified in any step below, all later files will be ignored (see *note Operating mode options::). The basic idea behind setting this progressive state of checking for parameter values is that separate users of a computer or separate folders in a user’s file system might need different values for some parameters. In each step, there can also be a configuration file containing the common options in all the programs: ‘gnuastro.conf’ (see *note Common options::). If options specific to one program are specified in this file, there will be un-recognized option errors, or unexpected behavior if the option has different behavior in another program. On the other hand, there is no problem with ‘astprogname.conf’ containing common options(1). 1. Command-line options, for a particular run of ProgramName. 2. ‘.gnuastro/astprogname.conf’ is parsed by ProgramName in the current directory. 3. ‘.gnuastro/gnuastro.conf’ is parsed by all Gnuastro programs in the current directory. 4. ‘$HOME/.local/etc/astprogname.conf’ is parsed by ProgramName in the user’s home directory (see *note Current directory and User wide::). 5. ‘$HOME/.local/etc/gnuastro.conf’ is parsed by all Gnuastro programs in the user’s home directory (see *note Current directory and User wide::). 6. ‘prefix/etc/astprogname.conf’ is parsed by ProgramName in the system-wide installation directory (see *note System wide:: for ‘prefix’). 7. ‘prefix/etc/gnuastro.conf’ is parsed by all Gnuastro programs in the system-wide installation directory (see *note System wide:: for ‘prefix’). *Manipulating the order:* You can manipulate this order or add new files with the following two options which are fully described in *note Operating mode options::: ‘--config’ Allows you to define any file to be parsed as a configuration file on the command-line or within the any other configuration file. Recall that the file given to ‘--config’ is parsed immediately when this option is confronted (on the command-line or in a configuration file). ‘--lastconfig’ Allows you to stop the parsing of subsequent configuration files. Note that if this option is given in a configuration file, it will be fully read, so its position in the configuration doesn’t matter (unlike ‘--config’). One example of benefiting from these configuration files can be this: raw telescope images usually have their main image extension in the second FITS extension, while processed FITS images usually only have one extension. If your system-wide default input extension is 0 (the first), then when you want to work with the former group of data you have to explicitly mention it to the programs every time. With this progressive state of default values to check, you can set different default values for the different directories that you would like to run Gnuastro in for your different purposes, so you won’t have to worry about this issue any more. The same can be said about the ‘gnuastro.conf’ files: by specifying a behavior in this single file, all Gnuastro programs in the respective directory, user, or system-wide steps will behave similarly. For example to keep the input’s directory when no specific output is given (see *note Automatic output::), or to not delete an existing file if it has the same name as a given output (see *note Input output options::). ---------- Footnotes ---------- (1) As an example, the ‘--setdirconf’ and ‘--setusrconf’ options will also write the common options they have read in their produced ‘astprogname.conf’.  File: gnuastro.info, Node: Current directory and User wide, Next: System wide, Prev: Configuration file precedence, Up: Configuration files 4.2.3 Current directory and User wide ------------------------------------- For the current (local) and user-wide directories, the configuration files are stored in the hidden sub-directories named ‘.gnuastro/’ and ‘$HOME/.local/etc/’ respectively. Unless you have changed it, the ‘$HOME’ environment variable should point to your home directory. You can check it by running ‘$ echo $HOME’. Each time you run any of the programs in Gnuastro, this environment variable is read and placed in the above address. So if you suddenly see that your home configuration files are not being read, probably you (or some other program) has changed the value of this environment variable. Although it might cause confusions like above, this dependence on the ‘HOME’ environment variable enables you to temporarily use a different directory as your home directory. This can come in handy in complicated situations. To set the user or current directory configuration files based on your command-line input, you can use the ‘--setdirconf’ or ‘--setusrconf’, see *note Operating mode options::.  File: gnuastro.info, Node: System wide, Prev: Current directory and User wide, Up: Configuration files 4.2.4 System wide ----------------- When Gnuastro is installed, the configuration files that are shipped with the distribution are copied into the (possibly system wide) ‘prefix/etc/’ directory. For more details on ‘prefix’, see *note Installation directory:: (by default it is: ‘/usr/local’). This directory is the final place (with the lowest priority) that the programs in Gnuastro will check to retrieve parameter values. If you remove an option and its value from the system wide configuration files, you either have to specify it in more immediate configuration files or set it each time in the command-line. Recall that none of the programs in Gnuastro keep any internal default values and will abort if they don’t find a value for the necessary parameters (except the number of threads and output file name). So even though you might never expect to use an optional option, it safe to have it available in this system-wide configuration file even if you don’t intend to use it frequently. Note that in case you install Gnuastro from your distribution’s repositories, ‘prefix’ will either be set to ‘/’ (the root directory) or ‘/usr’, so you can find the system wide configuration variables in ‘/etc/’ or ‘/usr/etc/’. The prefix of ‘/usr/local/’ is conventionally used for programs you install from source by your self as in *note Quick start::.  File: gnuastro.info, Node: Multi-threaded operations, Next: Numeric data types, Prev: Configuration files, Up: Common program behavior 4.3 Multi-threaded operations ============================= Some of the programs benefit significantly when you use all the threads your computer’s CPU has to offer to your operating system. The number of threads available can be larger than the number of physical (hardware) cores in the CPU (also known as Simultaneous multithreading). For example, in Intel’s CPUs (those that implement its Hyper-threading technology) the number of threads is usually double the number of physical cores in your CPU. On a GNU/Linux system, the number of threads available can be found with the command ‘$ nproc’ command (part of GNU Coreutils). Gnuastro’s programs can find the number of threads available to your system internally at run-time (when you execute the program). However, if a value is given to the ‘--numthreads’ option, the given number will be used, see *note Operating mode options:: and *note Configuration files:: for ways to use this option. Thus ‘--numthreads’ is the only common option in Gnuastro’s programs with a value that doesn’t have to be specified anywhere on the command-line or in the configuration files. * Menu: * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously.  File: gnuastro.info, Node: A note on threads, Next: How to run simultaneous operations, Prev: Multi-threaded operations, Up: Multi-threaded operations 4.3.1 A note on threads ----------------------- Spinning off threads is not necessarily the most efficient way to run an application. Creating a new thread isn’t a cheap operation for the operating system. It is most useful when the input data are fixed and you want the same operation to be done on parts of it. For example one input image to Crop and multiple crops from various parts of it. In this fashion, the image is loaded into memory once, all the crops are divided between the number of threads internally and each thread cuts out those parts which are assigned to it from the same image. On the other hand, if you have multiple images and you want to crop the same region(s) out of all of them, it is much more efficient to set ‘--numthreads=1’ (so no threads spin off) and run Crop multiple times simultaneously, see *note How to run simultaneous operations::. You can check the boost in speed by first running a program on one of the data sets with the maximum number of threads and another time (with everything else the same) and only using one thread. You will notice that the wall-clock time (reported by most programs at their end) in the former is longer than the latter divided by number of physical CPU cores (not threads) available to your operating system. Asymptotically these two times can be equal (most of the time they aren’t). So limiting the programs to use only one thread and running them independently on the number of available threads will be more efficient. Note that the operating system keeps a cache of recently processed data, so usually, the second time you process an identical data set (independent of the number of threads used), you will get faster results. In order to make an unbiased comparison, you have to first clean the system’s cache with the following command between the two runs. $ sync; echo 3 | sudo tee /proc/sys/vm/drop_caches *SUMMARY: Should I use multiple threads?* Depends: • If you only have *one* data set (image in most cases!), then yes, the more threads you use (with a maximum of the number of threads available to your OS) the faster you will get your results. • If you want to run the same operation on *multiple* data sets, it is best to set the number of threads to 1 and use Make, or GNU Parallel, as explained in *note How to run simultaneous operations::.  File: gnuastro.info, Node: How to run simultaneous operations, Prev: A note on threads, Up: Multi-threaded operations 4.3.2 How to run simultaneous operations ---------------------------------------- There are two(1) approaches to simultaneously execute a program: using GNU Parallel or Make (GNU Make is the most common implementation). The first is very useful when you only want to do one job multiple times and want to get back to your work without actually keeping the command you ran. The second is usually for more important operations, with lots of dependencies between the different products (for example a full scientific research). GNU Parallel When you only want to run multiple instances of a command on different threads and get on with the rest of your work, the best method is to use GNU parallel. Surprisingly GNU Parallel is one of the few GNU packages that has no Info documentation but only a Man page, see *note Info::. So to see the documentation after installing it please run $ man parallel As an example, let’s assume we want to crop a region fixed on the pixels (500, 600) with the default width from all the FITS images in the ‘./data’ directory ending with ‘sci.fits’ to the current directory. To do this, you can run: $ parallel astcrop --numthreads=1 --xc=500 --yc=600 ::: \ ./data/*sci.fits GNU Parallel can help in many more conditions, this is one of the simplest, see the man page for lots of other examples. For absolute beginners: the backslash (‘\’) is only a line breaker to fit nicely in the page. If you type the whole command in one line, you should remove it. Make Make is a program for building “targets†(e.g., files) using “recipes†(a set of operations) when their known “prerequisites†(other files) have been updated. It elegantly allows you to define dependency structures for building your final output and updating it efficiently when the inputs change. It is the most common infra-structure to build software today. Scientific research methodology is very similar to software development: you start by testing a hypothesis on a small sample of objects/targets with a simple set of steps. As you are able to get promising results, you improve the method and use it on a larger, more general, sample. In the process, you will confront many issues that have to be corrected (bugs in software development jargon). Make a wonderful tool to manage this style of development. It has been used to make reproducible papers, for example see the reproduction pipeline (https://gitlab.com/makhlaghi/NoiseChisel-paper) of the paper introducing *note NoiseChisel:: (one of Gnuastro’s programs). GNU Make(2) is the most common implementation which (similar to nearly all GNU programs, comes with a wonderful manual(3)). Make is very basic and simple, and thus the manual is short (the most important parts are in the first roughly 100 pages) and easy to read/understand. Make comes with a ‘--jobs’ (‘-j’) option which allows you to specify the maximum number of jobs that can be done simultaneously. For example if you have 8 threads available to your operating system. You can run: $ make -j8 With this command, Make will process your ‘Makefile’ and create all the targets (can be thousands of FITS images for example) simultaneously on 8 threads, while fully respecting their dependencies (only building a file/target when its prerequisites are successfully built). Make is thus strongly recommended for managing scientific research where robustness, archivability, reproducibility and speed(4) are very important. ---------- Footnotes ---------- (1) A third way would be to open multiple terminal emulator windows in your GUI, type the commands separately on each and press once on each terminal, but this is far too frustrating, tedious and prone to errors. It’s therefore not a realistic solution when tens, hundreds or thousands of operations (your research targets, multiplied by the operations you do on each) are to be done. (2) (3) (4) Besides its multi-threaded capabilities, Make will only re-build those targets that depend on a change you have made, not the whole work. For example, if you have set the prerequisites properly, you can easily test the changing of a parameter on your paper’s results without having to re-do everything (which is much faster). This allows you to be much more productive in easily checking various ideas/assumptions of the different stages of your research and thus produce a more robust result for your exciting science.  File: gnuastro.info, Node: Numeric data types, Next: Tables, Prev: Multi-threaded operations, Up: Common program behavior 4.4 Numeric data types ====================== At the lowest level, the computer stores everything in terms of ‘1’ or ‘0’. For example, each program in Gnuastro, or each astronomical image you take with the telescope is actually a string of millions of these zeros and ones. The space required to keep a zero or one is the smallest unit of storage, and is known as a _bit_. However, understanding and manipulating this string of bits is extremely hard for most people. Therefore, we define packages of these bits along with a standard on how to interpret the bits in each package as a _type_. The most basic standard for reading the bits is integer numbers ($..., -2, -1, 0, 1, 2, ...$, more bits will give larger limits). The common integer types are 8, 16, 32, and 64 bits wide. For each width, there are two standards for reading the bits: signed and unsigned integers. In the former, negative numbers are allowed and in the latter, they aren’t. The ‘unsigned’ types thus have larger positive limits (one extra bit), but no negative value. When the context of your work doesn’t involve negative numbers (for example counting, where negative is not defined), it is best to use the ‘unsigned’ types. For full numerical range of all integer types, see below. Another standard of converting a given number of bits to numbers is the floating point standard, this standard can approximately store any real number with a given precision. There are two common floating point types: 32-bit and 64-bit, for single and double precision floating point numbers respectively. The former is sufficient for data with less than 8 significant decimal digits (most astronomical data), while the latter is good for less than 16 significant decimal digits. The representation of real numbers as bits is much more complex than integers. If you are interested, you can start with the Wikipedia article (https://en.wikipedia.org/wiki/Floating_point). With the conversion operators in Gnuastro’s Arithmetic, you can change the types of data to each other, which is necessary in some contexts. For example the program/library, that you intend to feed the data into, only accepts floating point values, but you have an integer image. Another situation that conversion can be helpful is when you know that your data only has values that fit within ‘int8’ or ‘uint16’. However it is currently formatted in the ‘float64’ type. Operations involving floating point or larger integer types are significantly slower than integer or smaller-width types respectively. In the latter case, it also requires much more (by 8 or 4 times in the example above) storage space. So when you confront such situations and want to store/archive/transfter the data, it is best convert them to the most efficient type. The short and long names for the recognized numeric data types in Gnuastro are listed below. Both short and long names can be used when you want to specify a type. For example, as a value to the common option ‘--type’ (see *note Input output options::), or in the information comment lines of *note Gnuastro text table format::. The ranges listed below are inclusive. ‘u8’ ‘uint8’ 8-bit un-signed integers, range: $[0\rm{\ to\ }2^8-1]$ or $[0\rm{\ to\ }255]$. ‘i8’ ‘int8’ 8-bit signed integers, range: $[-2^7\rm{\ to\ }2^7-1]$ or $[-128\rm{\ to\ }127]$. ‘u16’ ‘uint16’ 16-bit un-signed integers, range: $[0\rm{\ to\ }2^{16}-1]$ or $[0\rm{\ to\ }65535]$. ‘i16’ ‘int16’ 16-bit signed integers, range: $[-2^{15}\rm{\ to\ }2^{15}-1]$ or $[-32768\rm{\ to\ }32767]$. ‘u32’ ‘uint32’ 32-bit un-signed integers, range: $[0\rm{\ to\ }2^{32}-1]$ or $[0\rm{\ to\ }4294967295]$. ‘i32’ ‘int32’ 32-bit signed integers, range: $[-2^{31}\rm{\ to\ }2^{31}-1]$ or $[-2147483648\rm{\ to\ }2147483647]$. ‘u64’ ‘uint64’ 64-bit un-signed integers, range $[0\rm{\ to\ }2^{64}-1]$ or $[0\rm{\ to\ }18446744073709551615]$. ‘i64’ ‘int64’ 64-bit signed integers, range: $[-2^{63}\rm{\ to\ }2^{63}-1]$ or $[-9223372036854775808\rm{\ to\ }9223372036854775807]$. ‘f32’ ‘float32’ 32-bit (single-precision) floating point types. The maximum (minimum is its negative) possible value is $3.402823\times10^{38}$. Single-precision floating points can accurately represent a floating point number up to $\sim7.2$ significant decimals. Given the heavy noise in astronomical data, this is usually more than sufficient for storing results. ‘f64’ ‘float64’ 64-bit (double-precision) floating point types. The maximum (minimum is its negative) possible value is $\sim10^{308}$. Double-precision floating points can accurately represent a floating point number $\sim15.9$ significant decimals. This is usually good for processing (mixing) the data internally, for example a sum of single precision data (and later storing the result as ‘float32’). *Some file formats don’t recognize all types.* Some file formats don’t recognize all the types, for example the FITS standard (see *note Fits::) does not define ‘uint64’ in binary tables or images. When a type is not acceptable for output into a given file format, the respective Gnuastro program or library will let you know and abort. On the command-line, you can use the *note Arithmetic:: program to convert the numerical type of a dataset, in the libraries, you can call ‘gal_data_copy_to_new_type’. gnuastro-0.5/doc/gnuastro.info0000644000175000017500000004667213217220437013445 00000000000000This is gnuastro.info, produced by makeinfo version 6.5 from gnuastro.texi. This book documents version 0.5 of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright © 2015-2017 Free Software Foundation, Inc. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled “GNU Free Documentation Licenseâ€. INFO-DIR-SECTION Astronomy START-INFO-DIR-ENTRY * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro’s library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. END-INFO-DIR-ENTRY  Indirect: gnuastro.info-1: 2942 gnuastro.info-2: 304058 gnuastro.info-3: 617914 gnuastro.info-4: 914677 gnuastro.info-5: 1203382  Tag Table: (Indirect) Node: Top2942 Node: Introduction22759 Node: Quick start25458 Node: Science and its tools28400 Ref: Science and its tools-Footnote-137876 Ref: Science and its tools-Footnote-237930 Ref: Science and its tools-Footnote-338075 Ref: Science and its tools-Footnote-438210 Node: Your rights38313 Ref: Your rights-Footnote-140635 Node: Naming convention40744 Node: Version numbering41881 Ref: Version numbering-Footnote-144958 Node: GNU Astronomy Utilities 1.045262 Ref: GNU Astronomy Utilities 1.0-Footnote-147203 Node: New to GNU/Linux?47235 Node: Command-line interface49199 Ref: Command-line interface-Footnote-154974 Ref: Command-line interface-Footnote-255006 Ref: Command-line interface-Footnote-355108 Node: Report a bug55344 Ref: Report a bug-Footnote-161189 Ref: Report a bug-Footnote-261252 Node: Suggest new feature61314 Node: Announcements64223 Node: Conventions64704 Node: Acknowledgments66391 Node: Tutorials69261 Ref: Tutorials-Footnote-170954 Node: Hubble visually checks and classifies his catalog71593 Ref: Hubble visually checks and classifies his catalog-Footnote-180313 Ref: Hubble visually checks and classifies his catalog-Footnote-280673 Ref: Hubble visually checks and classifies his catalog-Footnote-380913 Ref: Hubble visually checks and classifies his catalog-Footnote-481064 Ref: Hubble visually checks and classifies his catalog-Footnote-581308 Node: Sufi simulates a detection81354 Ref: Sufi simulates a detection-Footnote-1101250 Ref: Sufi simulates a detection-Footnote-2101544 Node: General program usage tutorial101922 Ref: General program usage tutorial-Footnote-1154382 Ref: General program usage tutorial-Footnote-2154460 Ref: General program usage tutorial-Footnote-3154505 Ref: General program usage tutorial-Footnote-4154550 Ref: General program usage tutorial-Footnote-5154631 Ref: General program usage tutorial-Footnote-6154768 Ref: General program usage tutorial-Footnote-7154900 Ref: General program usage tutorial-Footnote-8155116 Ref: General program usage tutorial-Footnote-9155219 Node: Installation155275 Ref: Installation-Footnote-1157850 Node: Dependencies157937 Node: Mandatory dependencies159315 Node: GNU Scientific Library161456 Node: CFITSIO162303 Ref: CFITSIO-Footnote-1165571 Node: WCSLIB165733 Ref: WCSLIB-Footnote-1167316 Ref: WCSLIB-Footnote-2167450 Node: Optional dependencies167536 Ref: Optional dependencies-Footnote-1172000 Node: Bootstrapping dependencies172279 Ref: Bootstrapping dependencies-Footnote-1178398 Ref: Bootstrapping dependencies-Footnote-2178671 Ref: Bootstrapping dependencies-Footnote-3179133 Ref: Bootstrapping dependencies-Footnote-4179439 Ref: Bootstrapping dependencies-Footnote-5179591 Node: Downloading the source179797 Node: Release tarball180781 Node: Version controlled source184013 Ref: Version controlled source-Footnote-1186947 Ref: 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Node: Operating mode options262760 Ref: Operating mode options-Footnote-1274621 Node: Configuration files274683 Ref: Configuration files-Footnote-1276669 Ref: Configuration files-Footnote-2276738 Node: Configuration file format276959 Node: Configuration file precedence279366 Ref: Configuration file precedence-Footnote-1283415 Node: Current directory and User wide283584 Node: System wide284849 Node: Multi-threaded operations286368 Node: A note on threads287822 Node: How to run simultaneous operations290386 Ref: How to run simultaneous operations-Footnote-1294332 Ref: How to run simultaneous operations-Footnote-2294732 Ref: How to run simultaneous operations-Footnote-3294777 Ref: How to run simultaneous operations-Footnote-4294829 Node: Numeric data types295360 Node: Tables304058 Node: Recognized table formats307382 Node: Gnuastro text table format312765 Ref: Gnuastro text table format-Footnote-1322176 Node: Selecting table columns322402 Node: Tessellation326284 Node: Getting help332035 Node: --usage334538 Node: --help335884 Node: Man pages339753 Node: Info340584 Node: help-gnuastro mailing list342999 Node: Automatic output344069 Node: Output headers346458 Node: Data containers350782 Node: Fits353617 Node: Invoking astfits358402 Node: HDU manipulation363086 Node: Keyword manipulation365385 Ref: Keyword manipulation-Footnote-1373951 Node: ConvertType374808 Node: Recognized file formats376224 Ref: Recognized file formats-Footnote-1383956 Node: Color384003 Node: Invoking astconvertt387096 Node: Table397185 Ref: Table-Footnote-1399928 Node: Invoking asttable400322 Node: Data manipulation404546 Node: Crop405277 Node: Crop modes407425 Node: Crop section syntax414721 Node: Blank pixels417769 Node: Invoking astcrop419447 Node: Crop options422943 Ref: Crop options-Footnote-1436045 Ref: Crop options-Footnote-2436119 Node: Crop output436167 Node: Arithmetic439030 Node: Reverse polish notation440262 Ref: Reverse polish notation-Footnote-1442974 Ref: Reverse polish notation-Footnote-2443030 Node: Arithmetic operators443144 Node: Invoking astarithmetic462173 Node: Convolve470267 Ref: Convolve-Footnote-1472917 Ref: Convolve-Footnote-2473129 Node: Spatial domain convolution473413 Ref: Spatial domain convolution-Footnote-1474658 Node: Convolution process474719 Node: Edges in the spatial domain476939 Ref: Edges in the spatial domain-Footnote-1480170 Ref: Edges in the spatial domain-Footnote-2480266 Node: Frequency domain and Fourier operations480347 Node: Fourier series historical background483112 Ref: epicycle484690 Ref: Fourier series historical background-Footnote-1487894 Ref: Fourier series historical background-Footnote-2487995 Node: Circles and the complex plane488353 Ref: iandtime492856 Ref: Circles and the complex plane-Footnote-1493102 Node: Fourier series493471 Ref: Fourier series-Footnote-1497612 Node: Fourier transform497709 Ref: Fourier transform-Footnote-1500784 Node: Dirac delta and comb501030 Node: Convolution theorem504434 Ref: Convolution theorem-Footnote-1508534 Node: Sampling theorem508595 Ref: samplingfreq511371 Ref: Sampling theorem-Footnote-1515492 Node: Discrete Fourier transform515637 Ref: Discrete Fourier transform-Footnote-1518957 Ref: Discrete Fourier transform-Footnote-2519071 Node: Fourier operations in two dimensions519204 Ref: Fourier operations in two dimensions-Footnote-1521992 Node: Edges in the frequency domain522157 Node: Spatial vs. Frequency domain525849 Node: Convolution kernel527407 Node: Invoking astconvolve530149 Node: Warp536679 Ref: Warp-Footnote-1540119 Ref: Warp-Footnote-2540263 Node: Warping basics540425 Ref: Warping basics-Footnote-1546360 Ref: Warping basics-Footnote-2546456 Ref: Warping basics-Footnote-3546519 Ref: Warping basics-Footnote-4546580 Ref: Warping basics-Footnote-5546630 Node: Merging multiple warpings546886 Node: Resampling548368 Ref: Resampling-Footnote-1552645 Ref: Resampling-Footnote-2552730 Ref: Resampling-Footnote-3552823 Ref: Resampling-Footnote-4552889 Node: Invoking astwarp552937 Node: Data analysis564227 Node: Statistics565032 Node: Histogram and Cumulative Frequency Plot566608 Ref: Histogram and Cumulative Frequency Plot-Footnote-1570785 Node: Sigma clipping570943 Node: Sky value575330 Node: Sky value definition577385 Ref: Sky value definition-Footnote-1580718 Ref: Sky value definition-Footnote-2581038 Node: Sky value misconceptions581142 Ref: Sky value misconceptions-Footnote-1583503 Ref: Sky value misconceptions-Footnote-2583774 Node: Quantifying signal in a tile583859 Ref: Quantifying signal in a tile-Footnote-1588670 Node: Invoking aststatistics588765 Ref: Invoking aststatistics-Footnote-1614696 Ref: Invoking aststatistics-Footnote-2614902 Node: NoiseChisel617914 Node: NoiseChisel changes after publication621449 Ref: NoiseChisel changes after publication-Footnote-1626402 Node: Invoking astnoisechisel626823 Node: General NoiseChisel options631777 Node: Detection options642188 Node: Segmentation options659317 Node: NoiseChisel output666366 Node: MakeCatalog669225 Ref: MakeCatalog-Footnote-1672635 Ref: MakeCatalog-Footnote-2672880 Ref: MakeCatalog-Footnote-3673338 Ref: MakeCatalog-Footnote-4673460 Node: Detection and catalog production673655 Ref: Detection and catalog production-Footnote-1677326 Node: Quantifying measurement limits677383 Ref: Quantifying measurement limits-Footnote-1689737 Ref: Quantifying measurement limits-Footnote-2689808 Ref: Quantifying measurement limits-Footnote-3689983 Ref: Quantifying measurement limits-Footnote-4690066 Node: Measuring elliptical parameters690192 Node: Adding new columns to MakeCatalog698655 Node: Invoking astmkcatalog703457 Node: MakeCatalog input files708324 Node: MakeCatalog general settings710679 Node: Upper-limit magnitude settings713936 Node: MakeCatalog output columns720070 Node: Match732023 Node: Invoking astmatch732838 Node: Modeling and fittings742540 Node: MakeProfiles743164 Node: Modeling basics745822 Node: Defining an ellipse746602 Ref: Defining an ellipse-Footnote-1749584 Ref: Defining an ellipse-Footnote-2749784 Node: PSF749844 Ref: PSF-Footnote-1754163 Node: Stars754343 Node: Galaxies754995 Ref: Galaxies-Footnote-1756280 Node: Sampling from a function756483 Node: Oversampling761238 Node: If convolving afterwards762605 Node: Flux Brightness and magnitude763801 Ref: Flux Brightness and magnitude-Footnote-1766530 Ref: Flux Brightness and magnitude-Footnote-2766594 Ref: Flux Brightness and magnitude-Footnote-3766801 Ref: Flux Brightness and magnitude-Footnote-4767180 Ref: Flux Brightness and magnitude-Footnote-5767333 Node: Profile magnitude767448 Node: Invoking astmkprof769257 Node: MakeProfiles catalog773047 Node: MakeProfiles profile settings779486 Ref: MakeProfiles profile settings-Footnote-1788381 Node: MakeProfiles output dataset788531 Ref: MakeProfiles output dataset-Footnote-1798654 Node: MakeProfiles log file799230 Node: MakeNoise800582 Node: Noise basics801268 Node: Photon counting noise802087 Ref: Photon counting noise-Footnote-1806503 Node: Instrumental noise806611 Node: Final noised pixel value807978 Node: Generating random numbers808409 Ref: Generating random numbers-Footnote-1813285 Ref: Generating random numbers-Footnote-2813387 Ref: Generating random numbers-Footnote-3813458 Node: Invoking astmknoise813793 Node: High-level calculations816417 Node: CosmicCalculator817208 Node: Distance on a 2D curved space818634 Ref: flatplane821408 Ref: sphereandplane823635 Ref: Distance on a 2D curved space-Footnote-1830371 Ref: Distance on a 2D curved space-Footnote-2830653 Ref: Distance on a 2D curved space-Footnote-3831117 Ref: Distance on a 2D curved space-Footnote-4831281 Node: Extending distance concepts to 3D831369 Node: Invoking astcosmiccal832891 Node: CosmicCalculator input options834974 Node: CosmicCalculator specific calculations835907 Node: Library841116 Node: Review of library fundamentals843369 Node: Headers845498 Ref: Headers-Footnote-1855680 Ref: Headers-Footnote-2855738 Ref: Headers-Footnote-3855935 Ref: Headers-Footnote-4856052 Ref: Headers-Footnote-5856158 Node: Linking856239 Ref: Linking-Footnote-1865661 Ref: Linking-Footnote-2865852 Ref: Linking-Footnote-3866134 Ref: Linking-Footnote-4866308 Ref: Linking-Footnote-5866564 Node: Summary and example on libraries866658 Node: BuildProgram870568 Node: Invoking astbuildprog872109 Node: Gnuastro library880317 Ref: Gnuastro library-Footnote-1884363 Node: Configuration information884502 Ref: Configuration information-Footnote-1887334 Node: Multithreaded programming887389 Ref: Multithreaded programming-Footnote-1890450 Ref: Multithreaded programming-Footnote-2890610 Node: Implementation of pthread_barrier890672 Node: Gnuastro's thread related functions893582 Node: Library data types899331 Node: Library blank values914677 Node: Library data container921212 Node: Generic data container922379 Ref: Generic data container-Footnote-1934488 Ref: Generic data container-Footnote-2934547 Ref: Generic data container-Footnote-3934625 Node: Dataset size and allocation934694 Node: Arrays of datasets941493 Node: Copying datasets943532 Node: Dimensions946840 Node: Linked lists953948 Ref: Linked lists-Footnote-1959030 Node: List of strings959429 Node: List of int32_t962530 Node: List of size_t966200 Ref: List of size_t-Footnote-1970601 Node: List of float970703 Node: List of double974317 Node: List of void978070 Node: Ordered list of size_t980785 Node: Doubly linked ordered list of size_t983819 Node: List of gal_data_t987341 Node: FITS files990188 Node: FITS macros errors filenames991988 Node: CFITSIO and Gnuastro types994082 Node: FITS HDUs996627 Node: FITS header keywords999211 Node: FITS arrays1010433 Node: FITS tables1016334 Node: World Coordinate System1020732 Node: Text files1028926 Node: Table input output1034650 Node: Arithmetic on datasets1044358 Node: Tessellation library1056589 Node: Independent tiles1060750 Node: Tile grid1075966 Node: Bounding box1087647 Node: Polygons1090807 Node: Qsort functions1096062 Node: Permutations1098894 Ref: Permutations-Footnote-11101678 Node: Matching1101967 Node: Statistical operations1106788 Node: Binary datasets1120321 Node: Convolution functions1130207 Ref: Convolution functions-Footnote-11133442 Node: Interpolation1133495 Node: Git wrappers1136622 Node: Cosmology library1138451 Node: Library demo programs1141765 Node: Library demo - reading a image1142712 Node: Library demo - inspecting neighbors1144885 Node: Library demo - multi-threaded operation1146639 Node: Library demo - reading and writing table columns1152066 Node: Developing1157717 Node: Why C1160058 Ref: Why C-Footnote-11166040 Ref: Why C-Footnote-21166070 Ref: Why C-Footnote-31166104 Ref: Why C-Footnote-41166137 Ref: Why C-Footnote-51166202 Ref: Why C-Footnote-61166401 Ref: Why C-Footnote-71166507 Ref: Why C-Footnote-81166581 Ref: Why C-Footnote-91166708 Ref: Why C-Footnote-101166754 Ref: Why C-Footnote-111166985 Node: Program design philosophy1167031 Ref: Program design philosophy-Footnote-11170104 Ref: Program design philosophy-Footnote-21170366 Ref: Program design philosophy-Footnote-31170474 Node: Coding conventions1170522 Ref: Coding conventions-Footnote-11182977 Ref: Coding conventions-Footnote-21183049 Ref: Coding conventions-Footnote-31183357 Ref: Coding conventions-Footnote-41183520 Node: Program source1183790 Node: Mandatory source code files1184899 Node: The TEMPLATE program1193164 Node: Documentation1195822 Node: Building and debugging1203382 Node: Test scripts1206328 Ref: Test scripts-Footnote-11208945 Ref: Test scripts-Footnote-21209103 Node: Developer's checklist1209292 Node: Gnuastro project webpage1210916 Ref: Gnuastro project webpage-Footnote-11215198 Ref: Gnuastro project webpage-Footnote-21215252 Ref: Gnuastro project webpage-Footnote-31215288 Node: Developing mailing lists1215413 Node: Contributing to Gnuastro1217676 Node: Copyright assignment1219677 Node: Commit guidelines1223552 Ref: Commit guidelines-Footnote-11228285 Node: Production workflow1228348 Ref: Production workflow-Footnote-11231265 Ref: Production workflow-Footnote-21231344 Ref: Production workflow-Footnote-31231427 Node: Forking tutorial1231509 Ref: Forking tutorial-Footnote-11236069 Ref: Forking tutorial-Footnote-21236320 Node: Gnuastro programs list1236426 Node: Other useful software1240467 Node: SAO ds91240949 Ref: SAO ds9-Footnote-11242128 Node: Viewing multiextension FITS images1242157 Node: PGPLOT1245452 Ref: PGPLOT-Footnote-11249048 Node: GNU Free Doc. License1249100 Node: Index1274436  End Tag Table  Local Variables: coding: utf-8 End: gnuastro-0.5/doc/genauthors0000755000175000017500000000522012723106172013013 00000000000000#! /bin/sh # # Update/create authors for the documentation. But only when there is a Git # repository. When there is no $(top_srcdir)/.git directory, rely on the # existing authors list. If the authors.texi file has for some reason been # deleted from the non version controlled source, then the book will not be # made (Texinfo will complain about a missing authors.texi). # # Call like this: # genauthors TOP_SRCDIR # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Mosè Giordano # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it under # the terms of the GNU General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # Gnuastro is distributed in the hope that it will be useful, but WITHOUT # ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or # FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for # more details. # # You should have received a copy of the GNU General Public License along # with Gnuastro. If not, see . # Status report echo "Generating authors list for documentation." # Only do the job if a .git directory exists in the top source directory # (recall that this script is also present in the tar-ball with no .git # directory and might be run from there) if [ -d $1/.git ]; then # We will need to import the `.mailmap' file from the source directory # temporarily to correct the changing emails (see the comments in # `.mailmap'). Note that this script is run from within the `doc/' # directory. The original `.mailmap' is in the `TOP_SRCDIR', so even # when the source and build directories are the same, there is no # problem. ln -s $1/.mailmap .mailmap # Do NOT test if authors.texi is newer than ../.git. In some cases the # list of authors is created empty when running make in top directory # (in particular "make -jN" with N > 1), so authors.texi needs to be # recreated anyway. git --git-dir=$1/.git shortlog --numbered --summary --email --no-merges \ | sed -e 's// /' -e 's/@/@@/' -e "s/è/@\`e/" \ | awk '{printf "%s %s (%s, %s)@*\n", $2, $3, $4, $1}' \ > $1/doc/authors.texi # Clean up: rm .mailmap # Check if the authors.texi file was actually written: if [ ! -s $1/doc/authors.texi ]; then echo "authors.texi is empty!" exit 1 fi else echo "No Git repository detected, leaving $1/doc/authors.texi unchanged." fi gnuastro-0.5/doc/gnuastro.texi0000644000175000017500000450433313217175767013477 00000000000000\input texinfo @c -*-texinfo-*- @c %**start of header @setfilename gnuastro.info @settitle GNU Astronomy Utilities @documentencoding UTF-8 @allowcodebreaks false @c@afourpaper @c %**end of header @include version.texi @include formath.texi @c So dashes and underscores can be used in HTMLs @allowcodebreaks true @c So function output type is printed on first line @deftypefnnewline on @c Use section titles in cross references, not node titles. @xrefautomaticsectiontitle on @c For the indexes: @syncodeindex vr cp @syncodeindex pg cp @c Copyright information: @copying This book documents version @value{VERSION} of the GNU Astronomy Utilities (Gnuastro). Gnuastro provides various programs and libraries for astronomical data manipulation and analysis. Copyright @copyright{} 2015-2017 Free Software Foundation, Inc. @quotation Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled ``GNU Free Documentation License''. @end quotation @end copying @c To include in the info directory. @dircategory Astronomy @direntry * Gnuastro: (gnuastro). GNU Astronomy Utilities. * libgnuastro: (gnuastro)Gnuastro library. Full Gnuastro library doc. * help-gnuastro: (gnuastro)help-gnuastro mailing list. Getting help. * bug-gnuastro: (gnuastro)Report a bug. How to report bugs * Arithmetic: (gnuastro)Arithmetic. Arithmetic operations on pixels. * astarithmetic: (gnuastro)Invoking astarithmetic. Options to Arithmetic. * BuildProgram: (gnuastro)BuildProgram. Compile and run programs using Gnuastro's library. * astbuildprog: (gnuastro)Invoking astbuildprog. Options to BuildProgram. * ConvertType: (gnuastro)ConvertType. Convert different file types. * astconvertt: (gnuastro)Invoking astconvertt. Options to ConvertType. * Convolve: (gnuastro)Convolve. Convolve an input file with kernel. * astconvolve: (gnuastro)Invoking astconvolve. Options to Convolve. * CosmicCalculator: (gnuastro)CosmicCalculator. For cosmological params. * astcosmiccal: (gnuastro)Invoking astcosmiccal. Options to CosmicCalculator. * Crop: (gnuastro)Crop. Crop region(s) from image(s). * astcrop: (gnuastro)Invoking astcrop. Options to Crop. * Fits: (gnuastro)Fits. View and manipulate FITS extensions and keywords. * astfits: (gnuastro)Invoking astfits. Options to Fits. * MakeCatalog: (gnuastro)MakeCatalog. Make a catalog from labeled image. * astmkcatalog: (gnuastro)Invoking astmkcatalog. Options to MakeCatalog. * MakeNoise: (gnuastro)MakeNoise. Make (add) noise to an image. * astmknoise: (gnuastro)Invoking astmknoise. Options to MakeNoise. * MakeProfiles: (gnuastro)MakeProfiles. Make mock profiles. * astmkprof: (gnuastro)Invoking astmkprof. Options to MakeProfiles. * NoiseChisel: (gnuastro)NoiseChisel. Detect signal in noise. * astnoisechisel: (gnuastro)Invoking astnoisechisel. Options to NoiseChisel. * Statistics: (gnuastro)Statistics. Get image Statistics. * aststatistics: (gnuastro)Invoking aststatistics. Options to Statistics. * Table: (gnuastro)Table. Read and write FITS binary or ASCII tables. * asttable: (gnuastro)Invoking asttable. Options to Table. * Warp: (gnuastro)Warp. Warp a dataset to a new grid. * astwarp: (gnuastro)Invoking astwarp. Options to Warp. @end direntry @c Print title information: @titlepage @title GNU Astronomy Utilities @subtitle Astronomical data manipulation and analysis programs and libraries @subtitle for version @value{VERSION}, @value{UPDATED} @author Mohammad Akhlaghi @page Gnuastro (source code, book and webpage) authors (sorted by number of commits): @quotation @include authors.texi @end quotation @vskip 0pt plus 1filll @insertcopying @page @quotation @* @* @* @* @* @* @* @* @* For myself, I am interested in science and in philosophy only because I want to learn something about the riddle of the world in which we live, and the riddle of man's knowledge of that world. And I believe that only a revival of interest in these riddles can save the sciences and philosophy from narrow specialization and from an obscurantist faith in the expert's special skill, and in his personal knowledge and authority; a faith that so well fits our `post-rationalist' and `post-critical' age, proudly dedicated to the destruction of the tradition of rational philosophy, and of rational thought itself. @author Karl Popper. The logic of scientific discovery. 1959. @end quotation @end titlepage @shortcontents @contents @c Online version top information. @ifnottex @node Top, Introduction, (dir), (dir) @top GNU Astronomy Utilities @insertcopying @ifhtml To navigate easily in this web page, you can use the @code{Next}, @code{Previous}, @code{Up} and @code{Contents} links in the top and bottom of each page. @code{Next} and @code{Previous} will take you to the next or previous topic in the same level, for example from chapter 1 to chapter 2 or vice versa. To go to the sections or subsections, you have to click on the menu entries that are there when ever a sub-component to a title is present. @end ifhtml @end ifnottex @menu * Introduction:: General introduction. * Tutorials:: Tutorials or Cookbooks. * Installation:: Requirements and installation. * Common program behavior:: Common behavior in all programs. * Data containers:: Tools to operate on extensions and tables. * Data manipulation:: Tools for basic image manipulation. * Data analysis:: Analyze images. * Modeling and fittings:: Make and fit models. * High-level calculations:: Physical calculations. * Library:: Gnuastro's library of useful functions. * Developing:: The development environment. * Gnuastro programs list:: List and short summary of Gnuastro. * Other useful software:: Installing other useful software. * GNU Free Doc. License:: GNU Free documentation license. * Index:: Index of terms @detailmenu --- The Detailed Node Listing --- Introduction * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production. Version numbering * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release New to GNU/Linux? * Command-line interface:: Introduction to the command-line Tutorials * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. * General program usage tutorial:: Usage of all programs in a good way. Installation * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. Dependencies * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source. Mandatory dependencies * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS. Downloading the source * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source. Version controlled source * Bootstrapping:: Adding all the automatically generated files. * Synchronizing:: Keep your local clone up to date. Build and install * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter. Configuring * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source. Common program behavior * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Multi-threaded operations:: How threads are managed in Gnuastro. * Numeric data types:: Different types and how to specify them. * Tables:: Recognized table formats. * Tessellation:: Tile the dataset into non-overlapping bins. * Getting help:: Getting more information on the go. * Automatic output:: About automatic output names. * Output headers:: Common headers to all FITS outputs. Command-line * Arguments and options:: Basics of options and arguments. * Common options:: Common options to all Gnuastro programs. Arguments and options * Arguments:: For specifying the main input files/operations. * Options:: For configuring the behavior of the program. Common options * Input output options:: Common input/output options. * Processing options:: Options for common processing steps. * Operating mode options:: Common operating mode options. Configuration files * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. Multi-threaded operations * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously. Tables * Recognized table formats:: Table formats that are recognized in Gnuastro. * Gnuastro text table format:: Gnuastro's convention plain text tables. * Selecting table columns:: Identify/select certain columns from a table Recognized table formats * Gnuastro text table format:: Reading plain text tables Getting help * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from --help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users. Data containers * Fits:: View and manipulate extensions and keywords. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text. Fits * Invoking astfits:: Arguments and options to Header. Invoking Fits * HDU manipulation:: Manipulate HDUs within a FITS file. * Keyword manipulation:: Manipulate metadata keywords in a HDU ConvertType * Recognized file formats:: Recognized file formats * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType. Table * Invoking asttable:: Options and arguments to Table. Data manipulation * Crop:: Crop region(s) from a dataset. * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * Warp:: Warp/Transform an image to a different grid. Crop * Crop modes:: Basic modes to define crop region. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astcrop:: Calling Crop on the command-line Invoking Crop * Crop options:: A list of all the options with explanation. * Crop output:: The outputs of Crop. Arithmetic * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output Convolve * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. Spatial domain convolution * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. Frequency domain and Fourier operations * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects. Warp * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astwarp:: Arguments and options for Warp. Data analysis * Statistics:: Calculate dataset statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. * Match:: Match two datasets. Statistics * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of @mymath{\sigma}-clipping. * Sky value:: Definition and derivation of the Sky value. * Invoking aststatistics:: Arguments and options to Statistics. Sky value * Sky value definition:: Definition of the Sky/reference value. * Sky value misconceptions:: Wrong methods to estimate the Sky value. * Quantifying signal in a tile:: Method to estimate the presence of signal. NoiseChisel * NoiseChisel changes after publication:: Changes to the software after publication. * Invoking astnoisechisel:: Options and arguments for NoiseChisel. Invoking NoiseChisel * General NoiseChisel options:: General NoiseChisel preprocessing. * Detection options:: Configure detection in NoiseChisel. * Segmentation options:: Configure segmentation in NoiseChisel. * NoiseChisel output:: NoiseChisel's output format. MakeCatalog * Detection and catalog production:: Discussing why/how to treat these separately * Quantifying measurement limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Adding new columns to MakeCatalog:: How to add new columns. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. Invoking MakeCatalog * MakeCatalog input files:: Specifying the different input files. * MakeCatalog general settings:: Options for general column settings. * Upper-limit magnitude settings:: Necessary to define upper-limit magnitudes. * MakeCatalog output columns:: How to specify the columns in the output. Match * Invoking astmatch:: Inputs, outputs and options of Match Modeling and fitting * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image. MakeProfiles * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles. Modeling basics * Defining an ellipse:: An ellipse on a pixelated grid. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model. Invoking MakeProfiles * MakeProfiles catalog:: Required catalog properties. * MakeProfiles profile settings:: Configuration parameters for all profiles. * MakeProfiles output dataset:: The canvas/dataset to build profiles over. * MakeProfiles log file:: A description of the optional log file. MakeNoise * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. Noise basics * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated. High-level calculations * CosmicCalculator:: Calculate cosmological variables CosmicCalculator * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator Invoking CosmicCalculator * CosmicCalculator input options:: Options to specify input conditions. * CosmicCalculator specific calculations:: Requesting specific outputs. Library * Review of library fundamentals:: Guide on libraries and linking. * BuildProgram:: Link and run source files with this library. * Gnuastro library:: Description of all library functions. * Library demo programs:: Demonstration for using libraries. Review of library fundamentals * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. BuildProgram * Invoking astbuildprog:: Options and examples for using this program. Gnuastro library * Configuration information:: General information about library config. * Multithreaded programming:: Tools for easy multi-threaded operations. * Library data types:: Definitions and functions for types. * Library blank values:: Blank values and functions to deal with them. * Library data container:: General data container in Gnuastro. * Dimensions:: Dealing with coordinates and dimensions. * Linked lists:: Various types of linked lists. * FITS files:: Working with FITS data. * World Coordinate System:: Dealing with the world coordinate system. * Text files:: Functions to work on Text files. * Table input output:: Reading and writing table columns. * Arithmetic on datasets:: Arithmetic operations on a dataset. * Tessellation library:: Functions for working on tiles. * Bounding box:: Finding the bounding box. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Permutations:: Re-order (or permute) the values in a dataset. * Matching:: Matching catalogs based on position. * Statistical operations:: Functions for basic statistics. * Binary datasets:: Datasets that can only have values of 0 or 1. * Convolution functions:: Library functions to do convolution. * Interpolation:: Interpolate (over blank values possibly). * Git wrappers:: Wrappers for functions in libgit2. * Cosmology library:: Cosmological calculations. Multithreaded programming (@file{threads.h}) * Implementation of pthread_barrier:: Some systems don't have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. Data container (@file{data.h}) * Generic data container:: Definition of Gnuastro's generic container. * Dataset size and allocation:: Functions for size and allocation. * Arrays of datasets:: Functions to help with array of datasets. * Copying datasets:: Functions to copy a dataset to a new one. Linked lists (@file{list.h}) * List of strings:: Simply linked list of strings. * List of int32_t:: Simply linked list of int32_ts. * List of size_t:: Simply linked list of size_ts. * List of float:: Simply linked list of floats. * List of double:: Simply linked list of doubles * List of void:: Simply linked list of void * pointers. * Ordered list of size_t:: Simply linked, ordered list of size_t. * Doubly linked ordered list of size_t:: Definition and functions. * List of gal_data_t:: Simply linked list Gnuastro's generic datatype. FITS files (@file{fits.h}) * FITS macros errors filenames:: General macros, errors and checking names. * CFITSIO and Gnuastro types:: Conversion between FITS and Gnuastro types. * FITS HDUs:: Opening and getting information about HDUs. * FITS header keywords:: Reading and writing FITS header keywords. * FITS arrays:: Reading and writing FITS images/arrays. * FITS tables:: Reading and writing FITS tables. Tessellation library (@file{tile.h}) * Independent tiles:: Work on or check independent tiles. * Tile grid:: Cover a full dataset with non-overlapping tiles. Library demo programs * Library demo - reading a image:: Read a FITS image into memory. * Library demo - inspecting neighbors:: Inspect the neighbors of a pixel. * Library demo - multi-threaded operation:: Doing an operation on threads. * Library demo - reading and writing table columns:: Simple Column I/O. Developing * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro's development. * Contributing to Gnuastro:: Share your changes with all users. Program source * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program. Contributing to Gnuastro * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git. Other useful software * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C SAO ds9 * Viewing multiextension FITS images:: Configure SAO ds9 for multiextension images. @end detailmenu @end menu @node Introduction, Tutorials, Top, Top @chapter Introduction @cindex GNU coding standards @cindex GNU Astronomy Utilities (Gnuastro) GNU Astronomy Utilities (Gnuastro) is an official GNU package consisting of separate programs and libraries for the manipulation and analysis of astronomical data. All the programs share the same basic command-line user interface for the comfort of both the users and developers. Gnuastro is written to comply fully with the GNU coding standards so it integrates finely with the GNU/Linux operating system. This also enables astronomers to expect a fully familiar experience in the source code, building, installing and command-line user interaction that they have seen in all the other GNU software that they use. The official and always up to date version of this book (or manual) is freely available under @ref{GNU Free Doc. License} in various formats (pdf, html, plain text, info, and as its Texinfo source) at @url{http://www.gnu.org/software/gnuastro/manual/}. For users who are new to the GNU/Linux environment, unless otherwise specified most of the topics in @ref{Installation} and @ref{Common program behavior} are common to all GNU software, for example installation, managing command-line options or getting help (also see @ref{New to GNU/Linux?}). So if you are new to this empowering environment, we encourage you to go through these chapters carefully. They can be a starting point from which you can continue to learn more from each program's own manual and fully benefit from and enjoy this wonderful environment. Gnuastro also comes with a large set of libraries, so you can write your own programs using Gnuastro's building blocks, see @ref{Review of library fundamentals} for an introduction. Finally it must be mentioned that in Gnuastro, no change to any program will be released before it has been fully documented in this here first. As discussed in @ref{Science and its tools} this is the founding basis of the Gnuastro. @menu * Quick start:: A quick start to installation. * Science and its tools:: Some philosophy and history. * Your rights:: User rights. * Naming convention:: About names of programs in Gnuastro. * Version numbering:: Understanding version numbers. * New to GNU/Linux?:: Suggested GNU/Linux distribution. * Report a bug:: Search and report the bug you found. * Suggest new feature:: How to suggest a new feature. * Announcements:: How to stay up to date with Gnuastro. * Conventions:: Conventions used in this book. * Acknowledgments:: People who helped in the production. @end menu @node Quick start, Science and its tools, Introduction, Introduction @section Quick start @cindex Test @cindex Check @cindex Build @cindex Compile @cindex GNU Tar @cindex Uncompress source @cindex Source, uncompress The latest official release tarball is always available as @url{http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.gz, @file{gnuastro-latest.tar.gz}}. For better compression (faster download), and robust archival features, an @url{http://www.nongnu.org/lzip/lzip.html, Lzip} compressed tarball is also available at @url{http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.lz, @file{gnuastro-latest.tar.lz}}, see @ref{Release tarball} for more details on the tarball release. @cindex Gzip @cindex Lzip @cindex GNU Tar The Gzip library and program are commonly available on most systems. However, Gnuastro recommends Lzip as described above and the beta-releases are also only distributed in @file{tar.lz}. You can download and install Lzip's source (in @file{.tar.gz} format) from its webpage and follow the same process as below: Lzip has no dependencies, so simply decompress, then run @command{./configure}, @command{make}, @command{sudo make install}. Let's assume the downloaded tarball is in the @file{TOPGNUASTRO} directory. The first two commands below can be used to decompress the source. If you download @file{tar.lz} and your Tar implementation doesn't recognize Lzip (the second command fails), run the third and fourth lines. Note that lines starting with @code{##} don't need to be typed. @example ## Go into the download directory. $ cd TOPGNUASTRO ## Also works on `tar.gz'. GNU Tar recognizes both formats. $ tar xf gnuastro-latest.tar.lz ## Only when previous command fails. $ lzip -d gnuastro-latest.tar.lz $ tar xf gnuastro-latest.tar @end example Gnuastro has three mandatory dependencies and some optional dependencies for extra functionality, see @ref{Dependencies} for the full list. Links to the dependency sources and instructions on installing each are fully described there. When the mandatory dependencies are ready, you can configure, compile, check and install Gnuastro on your system with the following commands. @example $ cd gnuastro-X.X # Replace X.X with version number. $ ./configure $ make -j8 # Replace 8 with no. CPU threads. $ make check $ sudo make install @end example @noindent See @ref{Known issues} if you confront any complications. For each program there is an `Invoke ProgramName' sub-section in this book which explains how the programs should be run on the command-line (for example @ref{Invoking asttable}). You can read the same section on the command-line by running @command{$ info astprogname} (for example @command{info asttable}). The `Invoke ProgramName' sub-section starts with a few examples of each program and goes on to explain the invocation details. See @ref{Getting help} for all the options you have to get help. In @ref{Tutorials} some real life examples of how these programs might be used are given. @node Science and its tools, Your rights, Quick start, Introduction @section Science and its tools History of science indicates that there are always inevitably unseen faults, hidden assumptions, simplifications and approximations in all our theoretical models, data acquisition and analysis techniques. It is precisely these that will ultimately allow future generations to advance the existing experimental and theoretical knowledge through their new solutions and corrections. In the past, scientists would gather data and process them individually to achieve an analysis thus having a much more intricate knowledge of the data and analysis. The theoretical models also required little (if any) simulations to compare with the data. Today both methods are becoming increasingly more dependent on pre-written software. Scientists are dissociating themselves from the intricacies of reducing raw observational data in experimentation or from bringing the theoretical models to life in simulations. These `intricacies' are precisely those unseen faults, hidden assumptions, simplifications and approximations that define scientific progress. @quotation @cindex Anscombe F. J. Unfortunately, most persons who have recourse to a computer for statistical analysis of data are not much interested either in computer programming or in statistical method, being primarily concerned with their own proper business. Hence the common use of library programs and various statistical packages. ... It's time that was changed. @author F. J. Anscombe. The American Statistician, Vol. 27, No. 1. 1973 @end quotation @cindex Anscombe's quartet @cindex Statistical analysis @url{http://en.wikipedia.org/wiki/Anscombe%27s_quartet,Anscombe's quartet} demonstrates how four data sets with widely different shapes (when plotted) give nearly identical output from standard regression techniques. Anscombe uses this (now famous) quartet, which was introduced in the paper quoted above, to argue that ``Good statistical analysis is not a purely routine matter, and generally calls for more than one pass through the computer''. Anscombe's quartet can be generalized to say that users of a software cannot claim to understand how it works only based on the experience they have gained by frequently using it. This kind of subjective experience is prone to very serious mis-understandings about the data, what the software/statistical-method really does (especially as it gets more complicated), and thus the scientific interpretation of the result. This attitude is further encouraged through non-free software@footnote{@url{https://www.gnu.org/philosophy/free-sw.html}}. This approach to scientific software only helps in producing dogmas and an ``obscurantist faith in the expert's special skill, and in his personal knowledge and authority''@footnote{Karl Popper. The logic of scientific discovery. 1959. Larger quote is given at the start of the PDF (for print) version of this book.}. @quotation @cindex Douglas Rushkoff Program or be programmed. Choose the former, and you gain access to the control panel of civilization. Choose the latter, and it could be the last real choice you get to make. @author Douglas Rushkoff. Program or be programmed, O/R Books (2010). @end quotation It is obviously impractical for any one human being to gain the intricate knowledge explained above for every step of an analysis. On the other hand, scientific data can be very large and numerous, for example images produced by telescopes in astronomy. This requires very efficient algorithms. To make things worse, natural scientists have generally not been trained in the advanced software techniques, paradigms and architecture that are taught in computer science or engineering courses and thus used in most software. The GNU Astronomy Utilities are an effort to tackle this issue. Gnuastro is not just a software, this book is as important to the idea behind Gnuastro as the source code (software). This book has tried to learn from the success of the ``Numerical Recipes'' book in educating those who are not software engineers and computer scientists but still heavy users of computational algorithms, like astronomers. There are two major differences: the code and the explanations are segregated: the code is moved within the actual Gnuastro software source code and the underlying explanations are given here. In the source code every non-trivial step is heavily commented and correlated with this book, it follows the same logic of this book, and all the programs follow a similar internal data, function and file structure, see @ref{Program source}. Complementing the code, this book focuses on thoroughly explaining the concepts behind those codes (history, mathematics, science, software and usage advise when necessary) along with detailed instructions on how to run the programs. At the expense of frustrating ``professionals'' or ``experts'', this book and the comments in the code also intentionally avoid jargon and abbreviations. The source code and this book are thus intimately linked, and when considered as a single entity can be thought of as a real (an actual software accompanying the algorithms) ``Numerical Recipes'' for astronomy. The other major and arguably more important difference is that ``Numerical Recipes'' does not allow you to distribute any code that you have learned from it. So while it empowers the privileged individual who has access to it, it exacerbates social ignorance. For example it does not allow you to release your software's source code if you have used their codes, you can only publicly release binaries (a black box) to the community. Exactly at the opposite end of the spectrum, Gnuastro's source code is released under the GNU general public license (GPL) and this book is released under the GNU free documentation license. You are therefore free to distribute any software you create using parts of Gnuastro's source code or text, or figures from this book, see @ref{Your rights}. While developing the source code and this book together, the developers of Gnuastro aim to impose the minimum requirements on you (in computer science, engineering and even the mathematics behind the tools) to understand and modify any step of Gnuastro if you feel the need to do so, see @ref{Why C} and @ref{Program design philosophy}. @cindex Galileo, G. Imagine if Galileo did not have the technical knowledge to build a telescope. Astronomical objects could not be seen with the Dutch military design of the telescope. In the beginning of his ``The Sidereal Messenger'' (1610) he cautions the readers on this issue and instructs them on how to build a suitable instrument: without a detailed description of ``how'' he made his observations, no one would believe him. The same is true today, science cannot progress with a black box. Before he actually saw the moons of Jupiter, the mountains on the Moon or the crescent of Venus, he was “evasive†to Kepler@footnote{Galileo G. (Translated by Maurice A. Finocchiaro). @emph{The essential Galileo}. Hackett publishing company, first edition, 2008.}. Science is not independent of its tools. @cindex Ken Thomson @cindex Stroustrup, Bjarne Bjarne Stroustrup (creator of the C++ language) says: ``Without understanding software, you are reduced to believing in magic''. Ken Thomson (the designer or the Unix operating system) says ``I abhor a system designed for the `user' if that word is a coded pejorative meaning `stupid and unsophisticated'.'' Certainly no scientist (user of a scientific software) would want to be considered a believer in magic, or `stupid and unsophisticated'. However, this can happen when scientists get too distant from the raw data and are mainly indulging themselves in their own high-level (abstract) models (creations). For example, roughly five years before special relativity and about two decades before quantum mechanics fundamentally changed Physics, Kelvin is quoted as saying: @quotation @cindex Lord Kelvin @cindex William Thomson There is nothing new to be discovered in physics now. All that remains is more and more precise measurement. @author William Thomson (Lord Kelvin), 1900 @end quotation @noindent A few years earlier, in a speech Albert. A. Michelson said: @quotation @cindex Albert. A. Michelson @cindex Michelson, Albert. A. The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decimals. @author Albert. A. Michelson, dedication of Ryerson Physics Lab, U. Chicago 1894 @end quotation @cindex Puzzle solving scientist @cindex Scientist, puzzle solver If scientists are considered to be more than mere ``puzzle solvers''@footnote{Thomas S. Kuhn. @emph{The Structure of Scientific Revolutions}, University of Chicago Press, 1962.} (simply adding to the decimals of known values or observing a feature in 10, 100, or 100000 more galaxies or stars, as Kelvin and Michelson clearly believed), they cannot just passively sit back and uncritically repeat the previous (observational or theoretical) methods/tools on new data. Today there is a wealth of raw telescope images ready (mostly for free) at the finger tips of anyone who is interested with a fast enough internet connection to download them. The only thing lacking is new ways to analyze this data and dig out the treasure that is lying hidden in them to existing methods and techniques. @quotation @cindex Jaynes E. T. New data that we insist on analyzing in terms of old ideas (that is, old models which are not questioned) cannot lead us out of the old ideas. However many data we record and analyze, we may just keep repeating the same old errors, missing the same crucially important things that the experiment was competent to find. @author Jaynes, Probability theory, the logic of science. Cambridge U. Press (2003). @end quotation @node Your rights, Naming convention, Science and its tools, Introduction @section Your rights @cindex GNU Texinfo The paragraphs below, in this section, belong to the GNU Texinfo@footnote{Texinfo is the GNU documentation system. It is used to create this book in all the various formats.} manual and are not written by us! The name ``Texinfo'' is just changed to ``GNU Astronomy Utilities'' or ``Gnuastro'' because they are released under the same licenses and it is beautifully written to inform you of your rights. @cindex Free software @cindex Copyright @cindex Public domain GNU Astronomy Utilities is ``free software''; this means that everyone is free to use it and free to redistribute it on certain conditions. Gnuastro is not in the public domain; it is copyrighted and there are restrictions on its distribution, but these restrictions are designed to permit everything that a good cooperating citizen would want to do. What is not allowed is to try to prevent others from further sharing any version of Gnuastro that they might get from you. Specifically, we want to make sure that you have the right to give away copies of the programs that relate to Gnuastro, that you receive the source code or else can get it if you want it, that you can change these programs or use pieces of them in new free programs, and that you know you can do these things. To make sure that everyone has such rights, we have to forbid you to deprive anyone else of these rights. For example, if you distribute copies of the Gnuastro related programs, you must give the recipients all the rights that you have. You must make sure that they, too, receive or can get the source code. And you must tell them their rights. Also, for our own protection, we must make certain that everyone finds out that there is no warranty for the programs that relate to Gnuastro. If these programs are modified by someone else and passed on, we want their recipients to know that what they have is not what we distributed, so that any problems introduced by others will not reflect on our reputation. @cindex GNU General Public License @cindex GNU Free Documentation License The precise conditions of the licenses for the programs currently being distributed that relate to Gnuastro are found in the @url{http://www.gnu.org/copyleft/gpl.html, GNU General Public license} that accompany them. This book is covered by the @url{http://www.gnu.org/copyleft/fdl.html, GNU Free Documentation License}. @node Naming convention, Version numbering, Your rights, Introduction @section Naming convention @cindex Names, programs @cindex Program names Gnuastro is a package of independent programs and a collection of libraries, here we are mainly concerned with the programs. Each program has an official name which consists of one or two words, describing what they do. The latter are printed with no space, for example NoiseChisel or Crop. On the command-line, you can run them with their executable names which start with an @file{ast} and might be an abbreviation of the official name, for example @file{astnoisechisel} or @file{astcrop}, see @ref{Executable names}. @pindex ProgramName @pindex @file{astprogname} We will use ``ProgramName'' for a generic official program name and @file{astprogname} for a generic executable name. In this book, the programs are classified based on what they do and thoroughly explained. An alphabetical list of the programs that are installed on your system with this installation are given in @ref{Gnuastro programs list}. That list also contains the executable names and version numbers along with a one line description. @node Version numbering, New to GNU/Linux?, Naming convention, Introduction @section Version numbering @cindex Version number @cindex Number, version @cindex Major version number @cindex Minor version number @cindex Mailing list: info-gnuastro Gnuastro can have two formats of version numbers, for official and unofficial releases. Official Gnuastro releases are announced on the @command{info-gnuastro} mailing list, they have a version control tag in Gnuastro's development history, and their version numbers are formatted like ``@file{A.B}''. @file{A} is a major version number, marking a significant planned achievement (for example see @ref{GNU Astronomy Utilities 1.0}), while @file{B} is a minor version number, see below for more on the distinction. Note that the numbers are not decimals, so version 2.34 is much more recent than version 2.5, which is not equal to 2.50. Gnuastro also allows a unique version number for unofficial releases. Unofficial releases can mark any point in Gnuastro's development history. This is done to allow astronomers to easily use any point in the version controlled history for their data-analysis and research publication. See @ref{Version controlled source} for a complete introduction. This section is not just for developers and is very straightforward, so please have a look if you are interested in the cutting-edge. This unofficial version number is a meaningful and easy to read string of characters, unique to that particular point of history. With this feature, users can easily stay up to date with the most recent bug fixes and additions that are committed between official releases. The unofficial version number is formatted like: @file{A.B.C-D}. @file{A} and @file{B} are the most recent official version number. @file{C} is the number of commits that have been made after version @file{A.B}. @file{D} is the first 4 or 5 characters of the commit hash number@footnote{Each point in Gnuastro's history is uniquely identified with a 40 character long hash which is created from its contents and previous history for example: @code{5b17501d8f29ba3cd610673261e6e2229c846d35}. So the string @file{D} in the version for this commit could be @file{5b17}, or @file{5b175}.}. Therefore, the unofficial version number `@code{3.92.8-29c8}', corresponds to the 8th commit after the official version @code{3.92} and its commit hash begins with @code{29c8}. The unofficial version number is sort-able (unlike the raw hash) and as shown above is very descriptive of the state of the unofficial release. Of course an official release is preferred for publication (since its tarballs are easily available and it has gone through more tests, making it more stable), so if an official release is announced prior to your publication's final review, please consider updating to the official release. The major version number is set by a major goal which is defined by the developers and user community before hand, for example see @ref{GNU Astronomy Utilities 1.0}. The incremental work done in minor releases are commonly small steps in achieving the major goal. Therefore, there is no limit on the number of minor releases and the difference between the (hypothetical) versions 2.927 and 3.0 can be a very small (negligible to the user) improvement that finalizes the defined goals. @menu * GNU Astronomy Utilities 1.0:: Plans for version 1.0 release @end menu @node GNU Astronomy Utilities 1.0, , Version numbering, Version numbering @subsection GNU Astronomy Utilities 1.0 @cindex Gnuastro major version number Currently (prior to Gnuastro 1.0), the aim of Gnuastro is to have a complete system for data manipulation and analysis at least similar to IRAF@footnote{@url{http://iraf.noao.edu/}}. So an astronomer can take all the standard data analysis steps (starting from raw data to the final reduced product and standard post-reduction tools) with the various programs in Gnuastro. @cindex Shell script The maintainers of each camera or detector on a telescope can provide a completely transparent shell script or Makefile to the observer for data analysis. This script can set configuration files for all the required programs to work with that particular camera. The script can then run the proper programs in the proper sequence. The user/observer can easily follow the standard shell script to understand (and modify) each step and the parameters used easily. Bash (or other modern GNU/Linux shell scripts) are very powerful and made for this gluing job. This will simultaneously improve performance and transparency. Shell scripting (or Makefiles) are also very basic constructs that are easy to learn and readily available as part of the Unix-like operating systems. If there is no program to do a desired step, Gnuastro's libraries can be used to build specific programs. The main factor is that all observatories or projects can freely contribute to Gnuastro and all simultaneously benefit from it (since it doesn't belong to any particular one of them), much like how for-profit organizations (for example RedHat, or Intel and many others) are major contributors to free and open source software for their shared benefit. Gnuastro's copyright has been fully awarded to GNU, so it doesn't belong to any particular astronomer or astronomical facility or project. @node New to GNU/Linux?, Report a bug, Version numbering, Introduction @section New to GNU/Linux? Some astronomers initially install and use the GNU/Linux operating systems because the software that their research community use can only be run in this environment, the transition is not necessarily easy. To encourage you in investing the patience and time to make this transition, we define the GNU/Linux system and argue for the command-line interface of scientific software and how it is worth the (apparently steep) learning curve. @ref{Command-line interface} contains a short overview of the very powerful command-line user interface. @ref{Tutorials} is a complete chapter with some real world example applications of Gnuastro making good use of GNU/Linux capabilities written for newcomers to this environment. It is fully explained, easy and (hopefully) entertaining. @cindex Linux @cindex GNU/Linux @cindex GNU C library @cindex GNU Compiler Collection You might have already noticed that we are not using the name ``Linux'', but ``GNU/Linux''. Please take the time to have a look at the following essays and FAQs for a complete understanding of this very important distinction. In short, the Linux kernel is built using the GNU C library (glibc) and GNU compiler collection (gcc). The Linux kernel software alone is useless, in order have an operating system you need many more packages and the majority of such low-level packages in most distributions are developed as part of the GNU project: ``the whole system is basically GNU with Linux loaded''. In the form of an analogy: to say “running Linuxâ€, is like saying “driving your carburetorâ€. @itemize @item @url{https://www.gnu.org/gnu/gnu-users-never-heard-of-gnu.html} @item @url{https://www.gnu.org/gnu/linux-and-gnu.html} @item @url{https://www.gnu.org/gnu/why-gnu-linux.html} @item @url{https://www.gnu.org/gnu/gnu-linux-faq.html} @end itemize @menu * Command-line interface:: Introduction to the command-line @end menu @node Command-line interface, , New to GNU/Linux?, New to GNU/Linux? @subsection Command-line interface @cindex Shell @cindex Graphic user interface @cindex Command-line user interface @cindex GUI: graphic user interface @cindex CLI: command-line user interface One aspect of Gnuastro that might be a little troubling to new GNU/Linux users is that (at least for the time being) it only has a command-line user interface (CLI). This might be contrary to the mostly graphical user interface (GUI) experience with proprietary operating systems. To a first time user, the command-line does appear much more complicated and adapting to it might not be easy and a little frustrating at first. This is understandable and also experienced by anyone who started using the computer (from childhood) in a graphical user interface. Here we hope to convince you of the unique benefits of this interface which can greatly enhance your productivity while complementing your GUI experience. @cindex GNOME 3 Through GNOME 3@footnote{@url{http://www.gnome.org/}}, most GNU/Linux based operating systems now have a very advanced and useful GUI. Since the GUI was created long after the command-line, some wrongly consider the command line to be obsolete. Both interfaces are very useful for different tasks (for example you can't view an image, video, pdf document or web page on the command-line!), on the other hand you can't reproduce your results easily in the GUI. Therefore they should not be regarded as rivals but as complementary user interfaces, here we will outline how the CLI can be useful in scientific programs. You can think of the GUI as a veneer over the CLI to facilitate a small subset of all the possible CLI operations. Each click you do on the GUI, can be thought of as internally running a different CLI command. So asymptotically (if a good designer can design a GUI which is able to show you all the possibilities to click on) the GUI is only as powerful as the command-line. In practice, such graphical designers are very hard to find for every program, so the GUI operations are always a subset of the internal CLI commands. For programs that are only made for the GUI, this results in not including lots of potentially useful operations. It also results in `interface design' to be a crucially important part of any GUI program. Scientists don't usually have enough resources to hire a graphical designer, also the complexity of the GUI code is far more than CLI code, which is harmful for a scientific software, see @ref{Science and its tools}. @cindex GUI: repeating operations For programs that have a GUI, one action on the GUI (moving and clicking a mouse, or tapping a touchscreen) might be more efficient and easier than its CLI counterpart (typing the program name and your desired configuration). However, if you have to repeat that same action more than once, the GUI will soon become very frustrating and prone to errors. Unless the designers of a particular program decided to design such a system for a particular GUI action, there is no general way to run any possible series of actions automatically on the GUI. @cindex GNU Bash @cindex Reproducible results @cindex CLI: repeating operations On the command-line, you can run any series of of actions which can come from various CLI capable programs you have decided your self in any possible permutation with one command@footnote{By writing a shell script and running it, for example see the tutorials in @ref{Tutorials}.}. This allows for much more creativity and exact reproducibility that is not possible to a GUI user. For technical and scientific operations, where the same operation (using various programs) has to be done on a large set of data files, this is crucially important. It also allows exact reproducibility which is a foundation principle for scientific results. The most common CLI (which is also known as a shell) in GNU/Linux is GNU Bash, we strongly encourage you to put aside several hours and go through this beautifully explained web page: @url{https://flossmanuals.net/command-line/}. You don't need to read or even fully understand the whole thing, only a general knowledge of the first few chapters are enough to get you going. Since the operations in the GUI are very limited and they are visible, reading a manual is not that important in the GUI (most programs don't even have any!). However, to give you the creative power explained above, with a CLI program, it is best if you first read the manual of any program you are using. You don't need to memorize any details, only an understanding of the generalities is needed. Once you start working, there are more easier ways to remember a particular option or operation detail, see @ref{Getting help}. @cindex GNU Emacs @cindex Virtual console To experience the command-line in its full glory and not in the GUI terminal emulator, press the following keys together: @key{CTRL+ALT+F4}@footnote{Instead of @key{F4}, you can use any of the keys from @key{F1} to @key{F6} for different virtual consoles depending on your GNU/Linux distribution, try them all out. You can also run a separate GUI from within this console if you want to.} to access the virtual console. To return back to your GUI, press the same keys above replacing @key{F4} with @key{F7} (or @key{F1}, or @key{F2}, depending on your GNU/Linux distribution). In the virtual console, the GUI, with all its distracting colors and information, is gone. Enabling you to focus entirely on your actual work. @cindex Resource heavy operations For operations that use a lot of your system's resources (processing a large number of large astronomical images for example), the virtual console is the place to run them. This is because the GUI is not competing with your research work for your system's RAM and CPU. Since the virtual consoles are completely independent, you can even log out of your GUI environment to give even more of your hardware resources to the programs you are running and thus reduce the operating time. @cindex Secure shell @cindex SSH @cindex Remote operation Since it uses far less system resources, the CLI is also very convenient for remote access to your computer. Using secure shell (SSH) you can log in securely to your system (similar to the virtual console) from anywhere even if the connection speeds are low. There are apps for smart phones and tablets which allow you to do this. @node Report a bug, Suggest new feature, New to GNU/Linux?, Introduction @section Report a bug @cindex Bug @cindex Wrong output @cindex Software bug @cindex Output, wrong @cindex Wrong results @cindex Results, wrong @cindex Halted program @cindex Program crashing @cindex Inconsistent results According to Wikipedia ``a software bug is an error, flaw, failure, or fault in a computer program or system that causes it to produce an incorrect or unexpected result, or to behave in unintended ways''. So when you see that a program is crashing, not reading your input correctly, giving the wrong results, or not writing your output correctly, you have found a bug. In such cases, it is best if you report the bug to the developers. The programs will also report bugs in known impossible situations (which are caused by something unexpected) and will ask the users to report the bug. @cindex Bug reporting Prior to actually filing a bug report, it is best to search previous reports. The issue might have already been found and even solved. The best place to check if your bug has already been discussed is the bugs tracker on @ref{Gnuastro project webpage} at @url{https://savannah.gnu.org/bugs/?group=gnuastro}. In the top search fields (under ``Display Criteria'') set the ``Open/Closed'' drop-down menu to ``Any'' and choose the respective program or general category of the bug in ``Category'' and click the ``Apply'' button. The results colored green have already been solved and the status of those colored in red is shown in the table. @cindex Version control Recently corrected bugs are probably not yet publicly released because they are scheduled for the next Gnuastro stable release. If the bug is solved but not yet released and it is an urgent issue for you, you can get the version controlled source and compile that, see @ref{Version controlled source}. To solve the issue as readily as possible, please follow the following to guidelines in your bug report. The @url{http://www.chiark.greenend.org.uk/~sgtatham/bugs.html, How to Report Bugs Effectively} and @url{http://catb.org/~esr/faqs/smart-questions.html, How To Ask Questions The Smart Way} essays also provide some very good generic advice for all software (don't contact their authors for Gnuastro's problems). Mastering the art of giving good bug reports (like asking good questions) can greatly enhance your experience with any free and open source software. So investing the time to read through these essays will greatly reduce your frustration after you see something doesn't work the way you feel it is supposed to for a large range of software, not just Gnuastro. @table @strong @item Be descriptive Please provide as many details as possible and be very descriptive. Explain what you expected and what the output was: it might be that your expectation was wrong. Also please clearly state which sections of the Gnuastro book (this book), or other references you have studied to understand the problem. This can be useful in correcting the book (adding links to likely places where users will check). But more importantly, it will be very encouraging for the developers, since you are showing how serious you are about the problem and that you have actually put some thought into it. ``To be able to ask a question clearly is two-thirds of the way to getting it answered.'' -- John Ruskin (1819-1900). @item Individual and independent bug reports If you have found multiple bugs, please send them as separate (and independent) bugs (as much as possible). This will significantly help us in managing and resolving them sooner. @cindex Reproducible bug reports @item Reproducible bug reports If we cannot exactly reproduce your bug, then it is very hard to resolve it. So please send us a Minimal working example@footnote{@url{http://en.wikipedia.org/wiki/Minimal_Working_Example}} along with the description. For example in running a program, please send us the full command-line text and the output with the @option{-P} option, see @ref{Operating mode options}. If it is caused only for a certain input, also send us that input file. In case the input FITS is large, please use Crop to only crop the problematic section and make it as small as possible so it can easily be uploaded and downloaded and not waste the archive's storage, see @ref{Crop}. @end table @noindent There are generally two ways to inform us of bugs: @itemize @cindex Mailing list archives @cindex Mailing list: bug-gnuastro @cindex @code{bug-gnuastro@@gnu.org} @item Send a mail to @code{bug-gnuastro@@gnu.org}. Any mail you send to this address will be distributed through the bug-gnuastro mailing list@footnote{@url{https://lists.gnu.org/mailman/listinfo/bug-gnuastro}}. This is the simplest way to send us bug reports. The developers will then register the bug into the project webpage (next choice) for you. @cindex Gnuastro project page @cindex Support request manager @cindex Submit new tracker item @cindex Anonymous bug submission @item Use the Gnuastro project webpage at @url{https://savannah.gnu.org/projects/gnuastro/}: There are two ways to get to the submission page as listed below. Fill in the form as described below and submit it (see @ref{Gnuastro project webpage} for more on the project webpage). @itemize @item Using the top horizontal menu items, immediately under the top page title. Hovering your mouse on ``Support'' will open a drop-down list. Select ``Submit new''. @item In the main body of the page, under the ``Communication tools'' section, click on ``Submit new item''. @end itemize @end itemize @cindex Tracker @cindex Bug tracker @cindex Task tracker @cindex Viewing trackers Once the items have been registered in the mailing list or webpage, the developers will add it to either the ``Bug Tracker'' or ``Task Manager'' trackers of the Gnuastro project webpage. These two trackers can only be edited by the Gnuastro project developers, but they can be browsed by anyone, so you can follow the progress on your bug. You are most welcome to join us in developing Gnuastro and fixing the bug you have found maybe a good starting point. Gnuastro is designed to be easy for anyone to develop (see @ref{Science and its tools}) and there is a full chapter devoted to developing it: @ref{Developing}. @node Suggest new feature, Announcements, Report a bug, Introduction @section Suggest new feature @cindex Feature requests @cindex Additions to Gnuastro We would always be very happy to hear of suggested new features. For every program there are already lists of features that we are planning to add. You can see the current list of plans from the Gnuastro project webpage at @url{https://savannah.gnu.org/projects/gnuastro/} and following @clicksequence{``Tasks''@click{}``Browse''} on the horizontal menu at the top of the page immediately under the title, see @ref{Gnuastro project webpage}. If you want to request a feature to an existing program, click on the ``Display Criteria'' above the list and under ``Category'', choose that particular program. Under ``Category'' you can also see the existing suggestions for new programs or other cases like installation, documentation or libraries. Also be sure to set the ``Open/Closed'' value to ``Any''. If the feature you want to suggest is not already listed in the task manager, then follow the steps that are fully described in @ref{Report a bug}. Please have in mind that the developers are all very busy with their own astronomical research, and implementing existing ``task''s to add or resolving bugs. Gnuastro is a volunteer effort and none of the developers are paid for their hard work. So, although we will try our best, please don't not expect that your suggested feature be immediately included (with the next release of Gnuastro). The best person to apply the exciting new feature you have in mind is you, since you have the motivation and need. In fact Gnuastro is designed for making it as easy as possible for you to hack into it (add new features, change existing ones and so on), see @ref{Science and its tools}. Please have a look at the chapter devoted to developing (@ref{Developing}) and start applying your desired feature. Once you have added it, you can use it for your own work and if you feel you want others to benefit from your work, you can request for it to become part of Gnuastro. You can then join the developers and start maintaining your own part of Gnuastro. If you choose to take this path of action please contact us before hand (@ref{Report a bug}) so we can avoid possible duplicate activities and get interested people in contact. @cartouche @noindent @strong{Gnuastro is a collection of low level programs:} As described in @ref{Program design philosophy}, a founding principle of Gnuastro is that each library or program should be very basic and low-level. High level jobs should be done by running the separate programs or using separate functions in succession through a shell script or calling the libraries by higher level functions, see the examples in @ref{Tutorials}. So when making the suggestions please consider how your desired job can best be broken into separate steps and modularized. @end cartouche @node Announcements, Conventions, Suggest new feature, Introduction @section Announcements @cindex Announcements @cindex Mailing list: info-gnuastro Gnuastro has a dedicated mailing list for making announcements. Anyone that is interested can subscribe to this mailing list to stay up to date with new releases or when the dependencies (see @ref{Dependencies}) have been updated. To subscribe to this list, please visit @url{https://lists.gnu.org/mailman/listinfo/info-gnuastro}. @node Conventions, Acknowledgments, Announcements, Introduction @section Conventions In this book we have the following conventions: @itemize @item All commands that are to be run on the shell (command-line) prompt as the user start with a @command{$}. In case they must be run as a super-user or system administrator, they will start with a single @command{#}. If the command is in a separate line and next line @code{is also in the code type face}, but doesn't have any of the @command{$} or @command{#} signs, then it is the output of the command after it is run. As a user, you don't need to type those lines. A line that starts with @command{##} is just a comment for explaining the command to a human reader and must not be typed. @item If the command becomes larger than the page width a @key{\} is inserted in the code. If you are typing the code by hand on the command-line, you don't need to use multiple lines or add the extra space characters, so you can omit them. If you want to copy and paste these examples (highly discouraged!) then the @key{\} should stay. The @key{\} character is a shell escape character which is used commonly to make characters which have special meaning for the shell loose that special place (the shell will not treat them specially if there is a @key{\} behind them). When it is a last character in a line (the next character is a new-line character) the new-line character looses its meaning an the shell sees it as a simple white-space character, enabling you to use multiple lines to write your commands. @end itemize @node Acknowledgments, , Conventions, Introduction @section Acknowledgments The list of Gnuastro authors is available at the start of this book and the @file{AUTHORS} file in the source code. Here the authors wish to gratefully acknowledge the help and support they received from other people and institutions who had an indirect (not committed in the version controlled history) role in Gnuastro. The plain text file @file{THANKS} which is distributed along with the source code also contains this list. The Japanese Ministry of Science and Technology (MEXT) scholarship for Mohammad Akhlaghi's Masters and PhD period in Tohoku University Astronomical Institute had an instrumental role in the long term learning and planning that made the idea of Gnuastro possible. The very critical view points of Professor Takashi Ichikawa (Mohammad's adviser) were also instrumental in the initial ideas and creation of Gnuastro. The European Research Council (ERC) advanced grant 339659-MUSICOS (Principal investigator: Roland Bacon) was vital in the growth and expansion of Gnuastro, enabling a thorough re-write of the core functionality of all libraries and programs, turning Gnuastro into the large collection of generic programs and libraries it is today. @c To the developers: please keep this in the same order as the THANKS file @c (alphabetical, except for the names in the paragraph above). In general, we would like to gratefully thank the following people for their useful and constructive comments and suggestions (in alphabetical order by family name): Marjan Akbari, Roland Bacon, Karl Berry, Leindert Boogaard, Nicolas Bouch@'e, Fernando Buitrago, Adrian Bunk, Rosa Calvi, Benjamin Clement, Antonio Diaz Diaz, Th@'er@`ese Godefroy, Madusha Gunawardhana, Stephen Hamer, Takashi Ichikawa, Ra@'ul Infante Sainz, Brandon Invergo, Aur@'elien Jarno, Lee Kelvin, Mohammad-Reza Khellat, Floriane Leclercq, Alan Lefor, Guillaume Mahler, Francesco Montanari, William Pence, Bob Proulx, Yahya Sefidbakht, Alejandro Serrano Borlaff, Lee Spitler, Richard Stallman, Ole Streicher, Alfred M. Szmidt, Ignacio Trujillo, David Valls-Gabaud and Christopher Willmer. The GNU French Translation Team is also managing the French version of the top Gnuastro webpage which we highly appreciate. Finally we should thank all the (sometimes anonymous) people in various online forums which patiently answered all our small (but important) technical questions. All work on Gnuastro has been voluntary, but the authors are most grateful to the following institutions (in chronological order) for hosting us in our research: @quotation Ministry of education, culture, sports, science and technology (MEXT), Japan.@* Tohoku University Astronomical Institute, Sendai, Japan.@* University of Salento, Lecce, Italy.@* Centre national de la recherche scientifique (CNRS), France.@* Centre de Recherche Astrophysique de Lyon, University of Lyon 1, France.@* @end quotation @node Tutorials, Installation, Introduction, Top @chapter Tutorials @cindex Tutorial @cindex Cookbook In this chapter we give several tutorials or cookbooks on how to use the various tools in Gnuastro for your scientific purposes. In these tutorials, we have intentionally avoided too many cross references to make it more easily readable. To get more information about a particular program, you can visit the section with the same name as the program in this book. Each program section starts by explaining the general concepts behind what it does. If you only want to see an explanation of the options and arguments of any program, see the subsection titled `Invoking ProgramName'. See @ref{Conventions}, for an explanation of the conventions we use in the example codes through the book. The tutorials in this section use a fictional setting of some historical figures in the history of astronomy. We have tried to show how Gnuastro would have been helpful for them in making their discoveries if there were GNU/Linux computers in their times! Please excuse us for any historical inaccuracy, this is not intended to be a historical reference. This form of presentation can make the tutorials more pleasant and entertaining to read while also being more practical (explaining from a user's point of view)@footnote{This form of presenting a tutorial was influenced by the PGF/TikZ and Beamer manuals. The first provides graphic capabilities, while with the second you can make presentation slides in @TeX{} and @LaTeX{}. In these manuals, Till Tantau (author of the manual) uses Euclid as the protagonist. There are also some nice words of wisdom for Unix-like systems called ``Rootless Root'': @url{http://catb.org/esr/writings/unix-koans/}. These also have a similar style but they use a mythical figure named Master Foo. If you already have some experience in Unix-like systems, you will definitely find these ``Unix Koans'' very entertaining.}. The main reference for the historical facts mentioned in these fictional settings was Wikipedia. @menu * Hubble visually checks and classifies his catalog:: Check a catalog. * Sufi simulates a detection:: Simulating a detection. * General program usage tutorial:: Usage of all programs in a good way. @end menu @node Hubble visually checks and classifies his catalog, Sufi simulates a detection, Tutorials, Tutorials @section Hubble visually checks and classifies his catalog @cindex Edwin Hubble In 1924 Hubble@footnote{Edwin Powell Hubble (1889 -- 1953 A.D.) was an American astronomer who can be considered as the father of extra-galactic astronomy, by proving that some nebulae are too distant to be within the Galaxy. He then went on to show that the universe appears to expand and also done a visual classification of the galaxies that is known as the Hubble fork.} announced his discovery that some of the known nebulous objects are too distant to be within the the Milky Way (or Galaxy) and that they were probably distant Galaxies@footnote{Note that at that time, ``Galaxy'' was a proper noun used to refer to the Milky way. The concept of a galaxy as we define it today had not yet become common. Hubble played a major role in creating today's concept of a galaxy.} in their own right. He had also used them to show that the redshift of the nebulae increases with their distance. So now he wants to study them more accurately to see what they actually are. Since they are nebulous or amorphous, they can't be modeled (like stars that are always a point) easily. So there is no better way to distinguish them than to visually inspect them and see if it is possible to classify these nebulae or not. Hubble has stored all the FITS images of the objects he wants to visually inspect in his @file{/mnt/data/images} directory. He has also stored his catalog of extra-galactic nebulae in @file{/mnt/data/catalogs/extragalactic.txt}. Any normal user on his GNU/Linux system (including himself) only has read access to the contents of the @file{/mnt/data} directory. He has done this by running this command as root: @example # chmod -R 755 /mnt/data @end example @noindent Hubble has done this intentionally to avoid mistakenly deleting or modifying the valuable images he has taken at Mount Wilson while he is working as an ordinary user. Retaking all those images and data is simply not an option. In fact they are also in another hard disk (@file{/dev/sdb1}). So if the hard disk which stores his GNU/Linux distribution suddenly malfunctions due to work load, his data is not in harms way. That hard disk is only mounted to this directory when he wants to use it with the command: @example # mount /dev/sdb1 /mnt/data @end example @noindent In short, Hubble wants to keep his data safe and fortunately by default Gnuastro allows for this. Hubble creates a temporary @file{visualcheck} directory in his home directory for this check. He runs the following commands to make the directory and change to it@footnote{The @code{pwd} command is short for ``Print Working Directory'' and @code{ls} is short for ``list'' which shows the contents of a directory.}: @example $ mkdir ~/visualcheck $ cd ~/visualcheck $ pwd /home/edwin/visualcheck $ ls @end example Hubble has multiple images in @file{/mnt/data/images}, some of his targets might be on the edges of an image and so several images need to be stitched to give a good view of them. Also his extra-galactic targets belong to various pointings in the sky, so they are not in one large image. Gnuastro's Crop is just the program he wants. The catalog in @file{extragalactic.txt} is a plain text file which stores the basic information of all his known 200 extra-galactic nebulae. In its second column it has each object's Right Ascension (the first column is a label he has given to each object) and in the third the object's declination. @example $ astcrop --coordcol=2 --coordcol=3 /mnt/data/images/*.fits \ --mode=wcs /mnt/data/catalogs/extragalactic.txt Crop started on Tue Jun 14 10:18:11 1932 ---- ./4_crop.fits 1 1 ---- ./2_crop.fits 1 1 ---- ./1_crop.fits 1 1 [[[ Truncated middle of list ]]] ---- ./198_crop.fits 1 1 ---- ./195_crop.fits 1 1 - 200 images created. - 200 were filled in the center. - 0 used more than one input. Crop finished in: 2.429401 (seconds) @end example @cindex Asynchronous thread allocation @noindent Hubble already knows that thread allocation to the the CPU cores is asynchronous. Hence each time you run it, the order of which job gets done first differs. When using Crop the order of outputs is irrelevant since each crop is independent of the rest. This is why the crops are not necessarily created in the same input order. He is satisfied with the default width of the outputs (which he inspected by running @code{$ astcrop -P}). If he wanted a different width for the cropped images, he could do that with the @option{--wwidth} option which accepts a value in arc-seconds. When he lists the contents of the directory again he finds his 200 objects as separate FITS images. @example $ ls 1_crop.fits 2_crop.fits ... 200_crop.fits @end example @cindex GNU Parallel The FITS image format was not designed for efficient/fast viewing, but mainly for accurate storing of the data. So he chooses to convert the cropped images to a more common image format to view them more quickly and easily through standard image viewers (which load much faster than FITS image viewer). JPEG is one of the most recognized image formats that is supported by most image viewers. Fortunately Gnuastro has just such a tool to convert various types of file types to and from each other: ConvertType. Hubble has already heard of GNU Parallel from one of his colleagues at Mount Wilson Observatory. It allows multiple instances of a command to be run simultaneously on the system, so he uses it in conjunction with ConvertType to convert all the images to JPEG. @example $ parallel astconvertt -ojpg ::: *_crop.fits @end example @pindex eog @cindex Eye of GNOME For his graphical user interface Hubble is using GNOME which is the default in most distributions in GNU/Linux. The basic image viewer in GNOME is the Eye of GNOME, which has the executable file name @command{eog} @footnote{Eye of GNOME is only available for users of the GNOME graphical desktop environment which is the default in most GNU/Linux distributions. If you use another graphical desktop environment, replace @command{eog} with any other image viewer.}. Since he has used it before, he knows that once it opens an image, he can use the @key{ENTER} or @key{SPACE} keys on the keyboard to go to the next image in the directory or the @key{Backspace} key to go the previous image. So he opens the image of the first object with the command below and with his cup of coffee in his other hand, he flips through his targets very fast to get a good initial impression of the morphologies of these extra-galactic nebulae. @example $ eog 1_crop.jpg @end example @cindex GNU Bash @cindex GNU Emacs @cindex Spiral galaxies @cindex Elliptical galaxies Hubble's cup of coffee is now finished and he also got a nice general impression of the shapes of the nebulae. He tentatively/mentally classified the objects into three classes while doing the visual inspection. One group of the nebulae have a very simple elliptical shape and seem to have no internal special structure, so he gives them code 1. Another clearly different class are those which have spiral arms which he associates with code 2 and finally there seems to be a class of nebulae in between which appear to have a disk but no spiral arms, he gives them code 3. Now he wants to know how many of the nebulae in his extra-galactic sample are within each class. Repeating the same process above and writing the results on paper is very time consuming and prone to errors. Fortunately Hubble knows the basics of GNU Bash shell programming, so he writes the following short script with a loop to help him with the job. After all, computers are made for us to operate and knowing basic shell programming gives Hubble this ability to creatively operate the computer as he wants. So using GNU Emacs@footnote{This can be done with any text editor} (his favorite text editor) he puts the following text in a file named @file{classify.sh}. @example for name in *.jpg do eog $name & processid=$! echo -n "$name belongs to class: " read class echo $name $class >> classified.txt kill $processid done @end example @cindex Gedit @cindex GNU Emacs Fortunately GNU Emacs or even simpler editors like Gedit (part of the GNOME graphical user interface) will display the variables and shell constructs in different colors which can really help in understanding the script. Put simply, the @code{for} loop gets the name of each JPEG file in the directory this script is run in and puts it in @code{name}. In the shell, the value of a variable is used by putting a @code{$} sign before the variable name. Then Eye of GNOME is run on the image in the background to show him that image and its process ID is saved internally (this is necessary to close Eye of GNOME later). The shell then prompts the user to specify a class and after saving it in @code{class}, it prints the file name and the given class in the next line of a file named @file{classified.txt}. To make the script executable (so he can run it later any time he wants) he runs: @example $ chmod +x classify.sh @end example @noindent Now he is ready to do the classification, so he runs the script: @example $ ./classify.sh @end example @noindent In the end he can delete all the JPEG and FITS files along with Crop's log file with the following short command. The only files remaining are the script and the result of the classification. @example $ rm *.jpg *.fits astcrop.txt $ ls classified.txt classify.sh @end example @noindent He can now use @file{classified.txt} as input to a plotting program to plot the histogram of the classes and start making interpretations about what these nebulous objects that are outside of the Galaxy are. @node Sufi simulates a detection, General program usage tutorial, Hubble visually checks and classifies his catalog, Tutorials @section Sufi simulates a detection It is the year 953 A.D. and Sufi@footnote{Abd al-rahman Sufi (903 -- 986 A.D.), also known in Latin as Azophi was an Iranian astronomer. His manuscript ``Book of fixed stars'' contains the first recorded observations of the Andromeda galaxy, the Large Magellanic Cloud and seven other non-stellar or `nebulous' objects.} is in Shiraz as a guest astronomer. He had come there to use the advanced 123 centimeter astrolabe for his studies on the Ecliptic. However, something was bothering him for a long time. While mapping the constellations, there were several non-stellar objects that he had detected in the sky, one of them was in the Andromeda constellation. During a trip he had to Yemen, Sufi had seen another such object in the southern skies looking over the Indian ocean. He wasn't sure if such cloud-like non-stellar objects (which he was the first to call `Sah@={a}bi' in Arabic or `nebulous') were real astronomical objects or if they were only the result of some bias in his observations. Could such diffuse objects actually be detected at all with his detection technique? He still had a few hours left until nightfall (when he would continue his studies on the ecliptic) so he decided to find an answer to this question. He had thoroughly studied Claudius Ptolemy's (90 -- 168 A.D) Almagest and had made lots of corrections to it, in particular in measuring the brightness. Using his same experience, he was able to measure a magnitude for the objects and wanted to simulate his observation to see if a simulated object with the same brightness and size could be detected in a simulated noise with the same detection technique. The general outline of the steps he wants to take are: @enumerate @item Make some mock profiles in an oversampled image. The initial mock image has to be oversampled prior to convolution or other forms of transformation in the image. Through his experiences, Sufi knew that this is because the image of heavenly bodies is actually transformed by the atmosphere or other sources outside the atmosphere (for example gravitational lenses) prior to being sampled on an image. Since that transformation occurs on a continuous grid, to best approximate it, he should do all the work on a finer pixel grid. In the end he can re-sample the result to the initially desired grid size. @item Convolve the image with a PSF image that is oversampled to the same value as the mock image. Since he wants to finish in a reasonable time and the PSF kernel will be very large due to oversampling, he has to use frequency domain convolution which has the side effect of dimming the edges of the image. So in the first step above he also has to build the image to be larger by at least half the width of the PSF convolution kernel on each edge. @item With all the transformations complete, the image should be re-sampled to the same size of the pixels in his detector. @item He should remove those extra pixels on all edges to remove frequency domain convolution artifacts in the final product. @item He should add noise to the (until now, noise-less) mock image. After all, all observations have noise associated with them. @end enumerate Fortunately Sufi had heard of GNU Astronomy Utilities from a colleague in Isfahan (where he worked) and had installed it on his computer a year before. It had tools to do all the steps above. He had used MakeProfiles before, but wasn't sure which columns he had chosen in his user or system wide configuration files for which parameters, see @ref{Configuration files}. So to start his simulation, Sufi runs MakeProfiles with the @option{-P} option to make sure what columns in a catalog MakeProfiles currently recognizes and the output image parameters. In particular, Sufi is interested in the recognized columns (shown below). @example $ astmkprof -P [[[ ... Truncated lines ... ]]] # Output: type float32 # Type of output: e.g., int16, float32, etc... naxis 1000,1000 # Number of pixels along first FITS axis. oversample 5 # Scale of oversampling (>0 and odd). [[[ ... Truncated lines ... ]]] # Columns, by info (see `--searchin'), or number (starting from 1): ccol 2 # Center along first FITS axis (horizontal). ccol 3 # Center along second FITS axis (vertical). fcol 4 # sersic (1), moffat (2), gaussian (3), # point (4), flat (5), circumference (6). rcol 5 # Effective radius or FWHM in pixels. ncol 6 # Sersic index or Moffat beta. pcol 7 # Position angle. qcol 8 # Axis ratio. mcol 9 # Magnitude. tcol 10 # Truncation in units of radius or pixels. [[[ ... Truncated lines ... ]]] @end example @noindent In Gnuastro, column counting starts from 1, so the columns are ordered such that the first column (number 1) can be an ID he specifies for each object (and MakeProfiles ignores), each subsequent column is used used for another property of the profile. It is also possible to use column names for the values of these options and change these defaults, but Sufi preferred to stick to the defaults. Fortunately MakeProfiles has the capability to also make the PSF which is to be used on the mock image and using the @option{--prepforconv} option, he can also make the mock image to be larger by the correct amount and all the sources to be shifted by the correct amount. For his initial check he decides to simulate the nebula in the Andromeda constellation. The night he was observing, the PSF had roughly a FWHM of about 5 pixels, so as the first row (profile), he defines the PSF parameters and sets the radius column (@code{rcol} above, fifth column) to @code{5.000}, he also chooses a Moffat function for its functional form. Remembering how diffuse the nebula in the Andromeda constellation was, he decides to simulate it with a mock S@'{e}rsic index 1.0 profile. He wants the output to be 500 pixels by 500 pixels, so he puts the mock profile in the center. Looking at his drawings of it, he decides a reasonable effective radius for it would be 40 pixels on this image pixel scale, he sets the axis ratio and position angle to approximately correct values too and finally he sets the total magnitude of the profile to 3.44 which he had accurately measured. Sufi also decides to truncate both the mock profile and PSF at 5 times the respective radius parameters. In the end he decides to put four stars on the four corners of the image at very low magnitudes as a visual scale. Using all the information above, he creates the catalog of mock profiles he wants in a file named @file{cat.txt} (short for catalog) using his favorite text editor and stores it in a directory named @file{simulationtest} in his home directory. [The @command{cat} command prints the contents of a file, short for concatenation. So please copy-paste the lines after ``@command{cat cat.txt}'' into @file{cat.txt} when the editor opens in the steps above it, note that there are 7 lines, first one starting with @key{#}]: @example $ mkdir ~/simulationtest $ cd ~/simulationtest $ pwd /home/rahman/simulationtest $ emacs cat.txt $ ls cat.txt $ cat cat.txt # Column 4: PROFILE_NAME [,str7] Radial profile's functional name 1 0.0000 0.0000 moffat 5.000 4.765 0.0000 1.000 30.000 5.000 2 250.00 250.00 sersic 40.00 1.000 -25.00 0.400 3.4400 5.000 3 50.000 50.000 point 0.000 0.000 0.0000 0.000 9.0000 0.000 4 450.00 50.000 point 0.000 0.000 0.0000 0.000 9.2500 0.000 5 50.000 450.00 point 0.000 0.000 0.0000 0.000 9.5000 0.000 6 450.00 450.00 point 0.000 0.000 0.0000 0.000 9.7500 0.000 @end example @noindent The zero-point magnitude for his observation was 18. Now he has all the necessary parameters and runs MakeProfiles with the following command: @example $ astmkprof --prepforconv --naxis=500,500 --zeropoint=18.0 cat.txt MakeProfiles started on Sat Oct 6 16:26:56 953 - 6 profiles read from cat.txt - Random number generator (RNG) type: mt19937 - Using 8 threads. ---- row 2 complete, 5 left to go ---- row 3 complete, 4 left to go ---- row 4 complete, 3 left to go ---- row 5 complete, 2 left to go ---- ./0_cat.fits created. ---- row 0 complete, 1 left to go ---- row 1 complete, 0 left to go - ./cat.fits created. 0.041651 seconds MakeProfiles finished in 0.267234 seconds $ls 0_cat.fits cat.fits cat.txt @end example @cindex Oversample @noindent The file @file{0_cat.fits} is the PSF Sufi had asked for and @file{cat.fits} is the image containing the other 5 objects. The PSF is now available to him as a separate file for the convolution step. While he was preparing the catalog, one of his students approached him and was also following the steps. When he opened the image, the student was surprised to see that all the stars are only one pixel and not in the shape of the PSF as we see when we image the sky at night. So Sufi explained to him that the stars will take the shape of the PSF after convolution and this is how they would look if we didn't have an atmosphere or an aperture when we took the image. The size of the image was also surprising for the student, instead of 500 by 500, it was 2630 by 2630 pixels. So Sufi had to explain why oversampling is very important for parts of the image where the flux change is significant over a pixel. Sufi then explained to him that after convolving we will re-sample the image to get our originally desired size. To convolve the image, Sufi ran the following command: @example $ astconvolve --kernel=0_cat.fits cat.fits Convolve started on Mon Apr 6 16:35:32 953 - Using 8 CPU threads. - Input: cat.fits (hdu: 1) - Kernel: 0_cat.fits (hdu: 1) - Input and Kernel images padded. 0.075541 seconds - Images converted to frequency domain. 6.728407 seconds - Multiplied in the frequency domain. 0.040659 seconds - Converted back to the spatial domain. 3.465344 seconds - Padded parts removed. 0.016767 seconds Convolve finished in: 10.422161 seconds $ls 0_cat.fits cat_convolved.fits cat.fits cat.txt @end example @noindent When convolution finished, Sufi opened the @file{cat_convolved.fits} file and showed the effect of convolution to his student and explained to him how a PSF with a larger FWHM would make the points even wider. With the convolved image ready, they were prepared to re-sample it to the original pixel scale Sufi had planned [from the @command{$ astmkprof -P} command above, recall that MakeProfiles had oversampled the image by 5 times]. Sufi explained the basic concepts of warping the image to his student and ran Warp with the following command: @example $ astwarp --scale=1/5 --centeroncorner cat_convolved.fits Warp started on Mon Apr 6 16:51:59 953 Using 8 CPU threads. Input: cat_convolved.fits (hdu: 1) matrix: 0.2000 0.0000 0.4000 0.0000 0.2000 0.4000 0.0000 0.0000 1.0000 $ ls 0_cat.fits cat_convolved_scaled.fits cat.txt cat_convolved.fits cat.fits $ astfits -p cat_convolved_scaled.fits | grep NAXIS NAXIS = 2 / number of data axes NAXIS1 = 526 / length of data axis 1 NAXIS2 = 526 / length of data axis 2 @end example @noindent @file{cat_convolved_warped.fits} now has the correct pixel scale. However, the image is still larger than what we had wanted, it is 526 (@mymath{500+13+13}) by 526 pixels. The student is slightly confused, so Sufi also resamples the PSF with the same scale and shows him that it is 27 (@mymath{2\times13+1}) by 27 pixels. Sufi goes on to explain how frequency space convolution will dim the edges and that is why he added the @option{--prepforconv} option to MakeProfiles, see @ref{If convolving afterwards}. Now that convolution is done, Sufi can remove those extra pixels using Crop with the command below. Crop's @option{--section} option accepts coordinates inclusively and counting from 1 (according to the FITS standard), so the crop's first pixel has to be 14, not 13. @example $ astcrop cat_convolved_scaled.fits --section=14:*-13,14:*-13 \ --zeroisnotblank Crop started on Sat Oct 6 17:03:24 953 - Read metadata of 1 image. 0.001304 seconds ---- ...nvolved_scaled_cropped.fits created: 1 input. Crop finished in: 0.027204 seconds $ls 0_cat.fits cat_convolved_scaled_cropped.fits cat.fits cat_convolved.fits cat_convolved_scaled.fits cat.txt @end example @noindent Finally, @file{cat_convolved_scaled_cropped.fits} has the same dimensions as Sufi had desired in the beginning. All this trouble was certainly worth it because now there is no dimming on the edges of the image and the profile centers are more accurately sampled. The final step to simulate a real observation would be to add noise to the image. Sufi set the zeropoint magnitude to the same value that he set when making the mock profiles and looking again at his observation log, he had measured the background flux near the nebula had a magnitude of 7 that night. So using these values he ran MakeNoise: @example $ astmknoise --zeropoint=18 --background=7 --output=out.fits \ cat_convolved_warped_crop.fits MakeNoise started on Mon Apr 6 17:05:06 953 - Generator type: mt19937 - Generator seed: 1428318100 MakeNoise finished in: 0.033491 (seconds) $ls 0_cat.fits cat_convolved_scaled_cropped.fits cat.fits out.fits cat_convolved.fits cat_convolved_scaled.fits cat.txt @end example @noindent The @file{out.fits} file now contains the noised image of the mock catalog Sufi had asked for. Seeing how the @option{--output} option allows the user to specify the name of the output file, the student was confused and wanted to know why Sufi hadn't used it before? Sufi then explained to him that for intermediate steps it is best to rely on the automatic output, see @ref{Automatic output}. Doing so will give all the intermediate files the same basic name structure, so in the end you can simply remove them all with the Shell's capabilities. So Sufi decided to show this to the student by making a shell script from the commands he had used before. The command-line shell has the capability to read all the separate input commands from a file. This is very useful when you want to do the same thing multiple times, with only the names of the files or minor parameters changing between the different instances. Using the shell's history (by pressing the up keyboard key) Sufi reviewed all the commands and then he retrieved the last 5 commands with the @command{$ history 5} command. He selected all those lines he had input and put them in a text file named @file{mymock.sh}. Then he defined the @code{edge} and @code{base} shell variables for easier customization later. Finally, before every command, he added some comments (lines starting with @key{#}) for future readability. @example # Basic settings: edge=13 base=cat # Remove any existing image to avoid confusion. rm out.fits # Run MakeProfiles to create an oversampled FITS image. astmkprof --prepforconv --naxis=500,500 --zeropoint=18.0 "$base".txt # Convolve the created image with the kernel. astconvolve --kernel=0_"$base".fits "$base".fits # Scale the image back to the intended resolution. astwarp --scale=1/5 --centeroncorner "$base"_convolved.fits # Crop the edges out (dimmed during convolution). `--section' accepts # inclusive coordinates, so the start of start of the section must be # one pixel larger than its end. st_edge=$(( edge + 1 )) astcrop "$base"_convolved_scaled.fits --zeroisnotblank \ --section=$st_edge:*-$edge,$st_edge:*-$edge # Add noise to the image. astmknoise --zeropoint=18 --background=7 --output=out.fits \ "$base"_convolved_scaled_cropped.fits # Remove all the temporary files. rm 0*.fits cat*.fits @end example @cindex Comments He used this chance to remind the student of the importance of comments in code or shell scripts: when writing the code, you have a very good mental picture of what you are doing, so writing comments might seem superfluous and excessive. However, in one month when you want to re-use the script, you have lost that mental picture and rebuilding it is can be very time-consuming and frustrating. The importance of comments is further amplified when you want to share the script with a friend/colleague. So it is very good to accompany any script/code with useful comments while you are writing it (have a good mental picture of what/why you are doing something). @cindex Gedit @cindex GNU Emacs Sufi then explained to the eager student that you define a variable by giving it a name, followed by an @code{=} sign and the value you want. Then you can reference that variable from anywhere in the script by calling its name with a @code{$} prefix. So in the script whenever you see @code{$base}, the value we defined for it above is used. If you use advanced editors like GNU Emacs or even simpler ones like Gedit (part of the GNOME graphical user interface) the variables will become a different color which can really help in understanding the script. We have put all the @code{$base} variables in double quotation marks (@code{"}) so the variable name and the following text do not get mixed, the shell is going to ignore the @code{"} after replacing the variable value. To make the script executable, Sufi ran the following command: @example $ chmod +x mymock.sh @end example @noindent Then finally, Sufi ran the script, simply by calling its file name: @example $ ./mymock.sh @end example After the script finished, the only file remaining is the @file{out.fits} file that Sufi had wanted in the beginning. Sufi then explained to the student how he could run this script anywhere that he has a catalog if the script is in the same directory. The only thing the student had to modify in the script was the name of the catalog (the value of the @code{base} variable in the start of the script) and the value to the @code{edge} variable if he changed the PSF size. The student was also very happy to hear that he won't need to make it executable again when he makes changes later, it will remain executable unless he explicitly changes the executable flag with @command{chmod}. The student was really excited, since now, through simple shell scripting, he could really speed up his work and run any command in any fashion he likes allowing him to be much more creative in his works. Until now he was using the graphical user interface which doesn't have such a facility and doing repetitive things on it was really frustrating and some times he would make mistakes. So he left to go and try scripting on his own computer. Sufi could now get back to his own work and see if the simulated nebula which resembled the one in the Andromeda constellation could be detected or not. Although it was extremely faint@footnote{The brightness of a diffuse object is added over all its pixels to give its final magnitude, see @ref{Flux Brightness and magnitude}. So although the magnitude 3.44 (of the mock nebula) is orders of magnitude brighter than 6 (of the stars), the central galaxy is much fainter. Put another way, the brightness is distributed over a large area in the case of a nebula.}, fortunately it passed his detection tests and he wrote it in the draft manuscript that would later become ``Book of fixed stars''. He still had to check the other nebula he saw from Yemen and several other such objects, but they could wait until tomorrow (thanks to the shell script, he only has to define a new catalog). It was nearly sunset and they had to begin preparing for the night's measurements on the ecliptic. @node General program usage tutorial, , Sufi simulates a detection, Tutorials @section General program usage tutorial @cindex HST @cindex XDF survey @cindex Hubble Space Telescope @cindex Extreme Deep Field survey Measuring colors of astronomical objects in broad-band or narrow-band images is one of the most basic and common steps in astronomical analysis. Here, we will use Gnuastro's programs to detect objects in a Hubble Space Telescope (HST) image and measure their colors. We will use the @url{https://archive.stsci.edu/prepds/xdf, eXtreme Deep Field} dataset. Like almost all astronomical surveys, this dataset is free for download and usable by the public. This tutorial was first prepared for the ``Exploring the Ultra-Low Surface Brightness Universe'' workshop (November 2017) at the International Space Science Institute (ISSI) in Bern, Switzerland. We would like to thank them and the attendees for a very fruitful week. You will need the following tools in this tutorial: Gnuastro, SAO DS9 @footnote{See @ref{SAO ds9}, available at @url{http://ds9.si.edu/site/Home.html}.}, GNU Wget@footnote{@url{https://www.gnu.org/software/wget}.}, and AWK (most common implementation is GNU AWK@footnote{@url{https://www.gnu.org/software/gawk}.}). @cartouche @noindent @strong{Type the example commands:} Try to type the example commands on your terminal and don't simply copy and paste them. This will help simulate future situations when you are processing your own datasets. @end cartouche A handy feature of Gnuastro is that all program names start with @code{ast}. This will allow your command-line processor to easily list and auto-complete Gnuastro's programs for you. Try typing the following command (press @key{TAB} key when you see @code{}) to see the list: @example $ ast @end example @noindent Any program that starts with @code{ast} (including all Gnuastro programs) will be shown. By choosing the subsequent characters of your desired program and pressing @key{} again, the list will narrow down and the program name will auto-complete once your input characters are unambiguous. In short, you often don't need to type the full name of the program you want to run. Gnuastro contains a large number of programs and it is natural to forget the details of each program's options. Therefore, before starting the analysis, let's review how you can refresh your memory any time you want on the command-line while working (without taking your hands off the keyboard). This book comes with your installation, so it will always correspond to your installed version of Gnuastro. Please see @ref{Info} for more. @cindex GNU Info GNU Info@footnote{GNU Info is already available on almost all Unix-like operating systems.} is the program in charge of displaying the manual on the command-line. To see this whole book on your command-line, please run the following command and subsequent keys. Info has its own mini-environment, therefore we'll show the keys that must be pressed in the mini-environment after a @code{->} sign. You can also ignore anything after the @code{#} sign in the middle of the line, they are only for your information. @example $ info gnuastro # Open the top of the manual. -> # All the book chapters. -> # Continue down: show sections. -> ... # Keep pressing space to go down. -> q # Quit Info, return to the command-line. @end example The thing that greatly simplifies navigation in Info is the links (regions with an underline). You can immediately go to the next link in the page with the @key{} key and press @key{} on it to go into that part of the manual. Try the commands above again, but this time also use @key{} to go to the links and press @key{} on them to go to the respective section of the book. Then follow a few more links and go deeper into the book. To return to the previous page, press @key{l} (small L). If you are searching for a specific phrase in the whole book (for example an option name), press @key{s} and type your search phrase and end it with an @key{}. You don't need to start from the top of the manual every time. For example, to get to @ref{Invoking astnoisechisel}, run the following command. In general, all programs have such an ``Invoking ProgramName'' section in this book. These sections are specifically for the description of inputs, outputs and configuration options of each program. You can access them directly for each program by giving its executable name to Info. @example $ info astnoisechisel @end example The other sections don't have such shortcuts. To directly access them from the command-line, you need to tell Info to look into Gnuastro's manual, then look for the specific section (an unambiguous title is necessary). For example, if you only want to review/remember NoiseChisel's @ref{Detection options} or @ref{Segmentation options}), just run any of these commands. Note how case is irrelevant for Info when calling a title in this manner. @example $ info gnuastro "Detection options" $ info gnuastro "segmentation options" @end example In general, Info is a wonderful and powerful way to access this whole book with detailed information about the programs you are running very fast. If you are not already familiar with it, please run the following command and just read along and do what it says to learn it. Don't stop until you feel have become sufficiently fluent in it. Please invest the half an hour's time necessary to start using Info comfortably. It will greatly improve your productivity and you will start reaping the rewards of this investment very soon. @example $ info info @end example As a good scientist you need to feel comfortable to play with the features/options and avoid (be critical to) using default values as much as possible. On the other hand, our human memory is very limited, so it is important to be able to easily access any part of this book fast and remember the option names, what they do and their acceptable values. If you just want the option names and a short description, calling the program with the @option{--help} option might also be a good solution like the first example below. If you know a few characters of the option name, you can feed the output to @command{grep} like the second or third example commands. @example $ astnoisechisel --help $ astnoisechisel --help | grep quant $ astnoisechisel --help | grep check @end example Let's start the processing. First, to keep things clean, let's create a @file{gnuastro-tutorial} directory and continue all future steps in it: @example $ mkdir gnuastro-tutorial $ cd gnuastro-tutorial @end example We will be using the near infra-red @url{http://www.stsci.edu/hst/wfc3, Wide Field Camera} dataset. If you already have them in another directory (for example @file{XDFDIR}), you can set the @file{download} directory to be a symbolic link to @file{XDFDIR} with a command like this: @example ln -s XDFDIR download @end example @noindent If the following images aren't already present on your system, you can make a @file{download} directory and download them there. @example $ mkdir download $ cd download $ xdfurl=http://archive.stsci.edu/pub/hlsp/xdf $ wget $xdfurl/hlsp_xdf_hst_wfc3ir-60mas_hudf_f105w_v1_sci.fits $ wget $xdfurl/hlsp_xdf_hst_wfc3ir-60mas_hudf_f160w_v1_sci.fits $ cd .. @end example @noindent In this tutorial, we'll just use these two filters. Later, you will probably need to download more filters, you can use the shell's @code{for} loop to download them all in series (one after the other@footnote{Note that you only have one port to the internet, so downloading in parallel will actually be slower than downloading in series.}) with one command like the one below for the WFC3 filters. Put this command instead of the two @code{wget} commands above. Recall that all the extra spaces, back-slashes (@code{\}), and new lines can be ignored if you are typing on the lines on the terminal. @example $ for f in f105w f125w f140w f160w; do \ wget $xdfurl/hlsp_xdf_hst_wfc3ir-60mas_hudf_"$f"_v1_sci.fits; \ done @end example First, let's visually inspect the dataset. Let's take F160W image as an example. Do the steps below with the other image(s) too (and later with any dataset that you want to work on). It is very important to understand your dataset visually. Note how ds9 doesn't follow the GNU style of options where ``long'' and ``short'' options are preceded by @option{--} and @option{-} respectively (for example @option{--width} and @option{-w}, see @ref{Options}). Ds9's @option{-zscale} option is a good scaling to highlight the low surface brightness regions, and as the name suggests, @option{-zoom to fit} will fit the whole dataset in the window. If the window is too small, expand it with your mouse, then press the ``zoom'' button on the top row of buttons above the image, then in the row below it, press ``zoom fit''. You can also zoom in and out by scrolling your mouse or the respective operation on your touch-pad when your cursor/pointer is over the image. @example $ ds9 download/hlsp_xdf_hst_wfc3ir-60mas_hudf_f160w_v1_sci.fits \ -zscale -zoom to fit @end example The first thing you might notice is that the regions with no data have a value of zero in this image. The next thing might be that the dataset actually has two ``depth''s (see @ref{Quantifying measurement limits}). The exposure time of the inner region is more than 4 times more than the outer parts. Fortunately the XDF survey webpage (above) contains the vertices of the deep flat WFC3-IR field. You can use those vertices in @ref{Crop} to cutout this deep infra-red region from the larger image. We'll make a directory called @file{flat-ir} and keep the flat infra-red regions in that directory (with a `@file{xdf-}' suffix for a shorter and easier filename). @example $ mkdir flat-ir $ astcrop --mode=wcs -h0 --output=flat-ir/xdf-f105w.fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" \ download/hlsp_xdf_hst_wfc3ir-60mas_hudf_f105w_v1_sci.fits $ astcrop --mode=wcs -h0 --output=flat-ir/xdf-f160w.fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" \ download/hlsp_xdf_hst_wfc3ir-60mas_hudf_f160w_v1_sci.fits @end example The only thing varying in the two calls to Gnuastro's Crop program is the filter name. Therefore, to simplify the command, and later allow work on more filters, we can use the shell's @code{for} loop. Notice how the two places where the filter names (@file{f105w} and @file{f160w}) are used above have been replaced with @file{$f} (the shell variable that @code{for} is in charge of setting) below. To generalize this for more filters later, you can simply add the other filter names in the first line before the semi-colon (@code{;}). @example $ for f in f105w f160w; do \ astcrop --mode=wcs -h0 --output=flat-ir/xdf-$f.fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" \ download/hlsp_xdf_hst_wfc3ir-60mas_hudf_"$f"_v1_sci.fits; \ done @end example Please open these images and inspect them with the same ds9 commands you used above. You will see how it is completely flat now and doesn't have varying depths. Another important result of this crop is that regions with no data now have a NaN (blank) value, not zero. Zero is a meaningful value and especially when using NoiseChisel, the input should have NaN values for pixels with no data, not zero. This is the deepest image we currently have of the sky. The first thing that comes to mind may be this: ``How large is this field?''. Let's find the answer to this question with the commands below. The lines starting with @code{##} are just comments for you to help in following the steps. Don't type them on the terminal. The commands are intentionally repetitive in some places to better understand each step and also to demonstrate the beauty of command-line features like variables, pipes and loops. Later, if you would like to repeat this process on another dataset, you can just use commands 3, 7, and 9. @cartouche @noindent @strong{Use shell history:} Don't forget to make effective use of your shell's history. This is especially convenient when you just want to make a small change to your previous command. Press the ``up'' key on your keyboard (possibly multiple times) to see your previous command(s). @end cartouche @example ## (1) See the general statistics of non-blank pixel values. $ aststatistics flat-ir/xdf-f160w.fits ## (2) We only want the number of non-blank pixels. $ aststatistics flat-ir/xdf-f160w.fits --number ## (3) Keep the result of the command above in the shell variable `n'. $ n=$(aststatistics flat-ir/xdf-f160w.fits --number) ## (4) See what is stored the shell variable `n'. $ echo $n ## (5) Show all the FITS keywords of this image. $ astfits flat-ir/xdf-f160w.fits -h1 ## (6) The resolution (in degrees/pixel) is in the `CDELT' keywords. ## Only show lines that contain these characters, by feeding ## the output of the previous command to the `grep' program. $ astfits flat-ir/xdf-f160w.fits -h1 | grep CDELT ## (7) Save the resolution (same in both dimensions) in the variable ## `r'. The last part uses AWK to print the third `field' of its ## input line. The first two fields were `CDELT1' and `='. $ r=$(astfits flat-ir/xdf-f160w.fits -h1 | grep CDELT1 \ | awk '@{print $3@}') ## (8) Print the values of `n' and `r'. $ echo $n $r ## (9) Use the number of pixels (first number passed to AWK) and ## length of each pixel's edge (second number passed to AWK) ## to estimate the area of the field in arc-minutes squared. $ area=(echo $n $r | awk '@{print $1 * ($2^2) * 3600@}') @end example The area of this field is 4.03817 (or 4.04) arc-minutes squared. Just for comparison, this is roughly 175 times smaller than the average moon's angular area (with a diameter of 30arc-minutes or half a degree). @cindex GNU AWK @cartouche @noindent @strong{AWK for table/value processing:} AWK is a powerful and simple tool for text processing. Above (and further below) some simple examples are shown. GNU AWK (the most common implementation) comes with a free and wonderful @url{https://www.gnu.org/software/gawk/manual/, book} in the same format as this book which will allow you to master it nicely. Just like this manual, you can also access GNU AWK's manual on the command-line whenever necessary without taking your hands off the keyboard as described above. @end cartouche This takes us to the second question that you have probably asked yourself when you saw the field for the first time: ``How large is this area at different redshifts?''. To get a feeling of the tangential area that this field covers at redshift 2, you can use @ref{CosmicCalculator}. In particular, you need the tangential distance covered by 1 arc-second as raw output. Combined with the field's area, we can then calculate the tangential distance in Mega Parsecs squared (@mymath{Mpc^2}). @example ## Print general cosmological properties at redshift 2. $ astcosmiccal -z2 ## When given a "Specific calculation" option, CosmicCalculator ## will just print that particular calculation. See the options ## under this title in the output of `--help' for more. $ astcosmiccal --help ## Only print the "Tangential dist. covered by 1arcsec at z (kpc)". ## in units of kpc/arc-seconds. $ astcosmiccal -z2 --arcsectandist ## Convert this distance to kpc^2/arcmin^2 and save in `k'. $ k=$(astcosmiccal -z2 --arcsectandist | awk '@{print ($1*60)^2@}') ## Multiply by the area of the field (in arcmin^2) and divide by ## 10^6 to return value in Mpc^2. $ echo $k $area | awk '@{print $1 * $2 / 1e6@}' @end example @noindent At redshift 2, this field therefore covers 1.07145 @mymath{Mpc^2}. If you would like to see how this tangential area changes with redshift, you can use a shell loop like below. @example $ for z in 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0; do \ k=$(astcosmiccal -z$z --arcsectandist); \ echo $z $k $area | awk '@{print $1, ($2*60)^2 * $3 / 1e6@}'; \ done @end example @noindent Fortunately, the shell has a very useful tool/program to print a sequence of numbers that is nicely called @code{seq}. You can use it instead of typing all the different redshifts in this example. For example the loop below will print the same range of redshifts (between 0.5 and 5) but with increments of 0.1. @example $ for z in $(seq 0.5 0.1 5); do \ k=$(astcosmiccal -z$z --arcsectandist); \ echo $z $k $area | awk '@{print $1, ($2*60)^2 * $3 / 1e6@}'; \ done @end example If you want a fast result and commonly need such processing for a larger number of redshifts, the command above can be slow. This is because the CosmicCalculator program has a lot of overhead: it has to parse the command-line and all configuration files (see below). These are both human-readable characters, not computer-readable bits. CosmicCalculator then has to check the sanity of its inputs and check which of its many options you have asked for. It has to do all of these for every redshift. To greatly speed up the processing, Gnuastro gives you direct access to the root work-horse of CosmicCalculator without all that overhead: @ref{Gnuastro library}. Using Gnuastro's library, you can write your own tiny little program for this same calculation, without all that extra overhead of CosmicCalculator (or any of Gnuastro's programs, see @ref{Library}). For this particular job, you want Gnuastro's @ref{Cosmology library}. Here is one example: put the following small C program in a file called @file{myprogram.c}. @example #include #include #include #include int main(void) @{ double area=4.03817; /* Area of field (arcmin^2). */ double z, adist, tandist; /* Temporary variables. */ /* Constants from Plank 2015 (Paper XIII, A&A 594, 2016) */ double H0=67.74, olambda=0.6911, omatter=0.3089, oradiation=0; /* Do the same thing for all redshifts (z) between 0.1 and 5. */ for(z=0.1; z<5; z+=0.1) @{ /* Calculate the angular diameter distance. */ adist=gal_cosmology_angular_distance(z, H0, olambda, omatter, oradiation); /* Calculate the tangential distance of one arcsecond. */ tandist = adist * 1000 * M_PI / 3600 / 180; /* Print the redshift and area. */ printf("%-5.2f %g\n", z, pow(tandist * 60,2) * area / 1e6); @} /* Tell the system that everything finished successfully. */ return EXIT_SUCCESS; @} @end example @noindent To build and run this C program, you can use @ref{BuildProgram}. It is designed to manage Gnuastro's dependencies, compile the program you give it and then run it. In short, it hides all the complexities of compiling, linking and running C programs based on Gnuastro's library. The library will later be usable higher level languages like Python or Julia, for now it is only usable by C and C++ programs. @example $ astbuildprog myprogram.c @end example See how much faster this is compared to the shell loop we wrote above? You might have noticed that a new file called @file{myprogram} is also created in the directory. This is the compiled program that was created and run by the command above (its in binary machine code, not human-readable any more). You can run it again to get the same results with a command like this: @example $ ./myprogram @end example The efficiency of @file{myprogram} compared to CosmicCalculator is because the requested processing is faster/comparable to the overheads. For other programs that take large input datasets (images for example), the overhead is usually negligible compared to the processing. In such cases, the libraries are only useful if you want a different/new processing compared to the functionalities in Gnuastro's existing programs. Gnuastro has a large library which all the programs use for various steps their processing. For the full list of available functions classified by context, please see @ref{Gnuastro library}. Gnuastro's library and BuildProgram are created to make it easy for you to use these powerful features and get to your scientific results as efficiently (fast) and accurately as possible. Several other complete working examples (involving images and tables) of Gnuastro's libraries can be see in @ref{Library demo programs}. We'll stop with the libraries at this point in this tutorial and get back to Gnuastro's already built programs which ready to be used on the command-line. None of Gnuastro's programs keep a default value internally within their code. However, when you ran CosmicCalculator with the @option{-z2} option above, it completed its processing and printed results. So where did the ``default'' cosmological parameter values (like the matter density and etc) come from? The values come from the command-line or a configuration file (see @ref{Configuration file precedence}). CosmicCalculator has a very limited set of parameters and doesn't need any particular file inputs. Therefore, we'll use it to discuss configuration files which are an important part of all Gnuastro's programs (see @ref{Configuration files}). Once you get comfortable with configuration files, you can easily do the same for the options of all Gnuastro programs. For example, NoiseChisel has the largest number of options in the programs. Therefore configuration files will be very useful for it when you use different datasets (with different noise properties or in different research contexts). The configuration of each program (besides its version) is vital for the reproducibility of your results, so it is very important to manage them properly. As we saw above, the full list of the options in all Gnuastro programs can be seen with the @option{--help} option. Try calling it with CosmicCalculator as shown below. Note how options are grouped by context to make it easier to find your desired option. However, in each group, options are ordered alphabetically. @example $ astcosmiccal --help @end example @noindent The options that need a value have an @key{=} sign after their long version and @code{FLT}, @code{INT} or @code{STR} for floating point numbers, integer numbers and strings (filenames for example) respectively. All options have a long format and some have a short format (a single character), for more see @ref{Options}. When you are using a program, it is often necessary to check the value the option has just before the program starts its processing. In other words, after it has parsed the command-line options and all configuration files. You can see the values of all options that need one with the @option{--printparams} or @code{-P} option that is common to all programs (see @ref{Common options}). In the command below, try replacing @code{-P} with @option{--printparams} to see how both do the same operation. @example $ astcosmiccal -P @end example Let's say you want a different Hubble constant. Try running the following command to see how the Hubble constant in the output of the command above has changed. Afterwards, delete the @option{-P} and add a @option{-z2} to see the results with the new cosmology (or configuration). @example $ astcosmiccal -P --H0=70 @end example From the output of the @code{--help} option, note how the option for Hubble constant has both short (@code{-H}) and long (@code{--H0}) formats. One final note is that the equal (@key{=}) sign is not mandatory. In the short format, the value can stick to the actual option (the short option name is just one character after-all and thus easily identifiable) and in the long format, a white-space character is also enough. @example $ astcosmiccal -H70 -z2 $ astcosmiccal --H0 70 -z2 --arcsectandisk @end example Let's assume that in one project, you want to only use rounded cosmological parameters (H0 of 70km/s/Mpc and matter density of 0.3). You should therefore run CosmicCalculator like this: @example $ astcosmiccal --H0=70 --olambda=0.7 --omatter=0.3 -z2 @end example But having to type these extra options every time you run CosmicCalculator will be prone to errors (typos in particular) and also will be frustrating and slow. Therefore in Gnuastro, you can put all the options and their values in a ``Configuration file'' and tell the programs to read the option values from there. Let's create a configuration file. In your favorite text editor, make a file named @file{my-cosmology.conf} (or @file{my-cosmology.txt}, the suffix doesn't matter) which contains the following lines. One space between the option value and name is enough, the values are just under each other to help in readability. Also note that you can only use long option names in configuration files. @example H0 70 olambda 0.7 omatter 0.3 @end example @noindent You can now tell CosmicCalculator to read this file for option values immediately using the @option{--config} option as shown below. Do you see how the output of the following command corresponds to the option values in @file{my-cosmology.txt} (previous command)? @example $ astcosmiccal --config=my-cosmology.conf -z2 @end example If you need this cosmology every time you are working in a specific directory, you can benefit from Gnuastro's default configuration files to avoid having to call the @option{--config} option. Let's assume that you want any CosmicCalculator call you make in the @file{my-cosmology} directory to use these parameters. You just have to copy the above configuration file into a special directory and file: @example $ mkdir my-cosmology $ mkdir my-cosmology/.gnuastro $ mv my-cosmology.conf my-cosmology/.gnuastro/astcosmiccal.conf @end example Once you run CosmicCalculator within @file{my-cosmology} as shown below, you will see how your cosmology has been implemented without having to type anything extra on the command-line. @example $ cd my-cosmology $ astcosmiccal -z2 $ cd .. @end example To further simplify the process, you can use the @option{--setdirconf} option. If you are already in your desired directory, calling this option with the others will automatically write the final values (along with descriptions) in @file{.gnuastro/astcosmiccal.conf}. For example the commands below will make the same configuration file automatically (with one extra call to CosmicCalculator). @example $ mkdir my-cosmology2 $ cd my-cosmology2 $ astcosmiccal --H0 70 --olambda=0.7 --omatter=0.3 --setdirconf $ astcosmiccal -z2 $ cd .. @end example Gnuastro's programs also have default configuration files for a specific user (when run in any directory). This allows you to set a special behavior every time a program is run by a specific user. Only the directory and filename differ from the above, the rest of the process is similar to before. Finally, there are also system-wide configuration files that can be used to define the option values for all users on a system. See @ref{Configuration file precedence} for a more detailed discussion. We are now ready to start processing the downloaded images. Since these datasets are already aligned, you don't need to align them to make sure the pixel grid covers the same region in all inputs. Gnuastro's Warp program has features for such pixel-grid warping (see @ref{Warp}). Therefore, just for a demonstration, let's assume one image needs to be rotated by 20 degrees to correspond to the other. To do that, you can run the following command: @example $ astwarp flat-ir/xdf-f160w.fits --rotate=20 @end example @noindent Open the output and see the output. If your final image is already aligned with RA and Dec, you can simply use the @option{--align} option and let Warp calculate the necessary rotation. Warp can generally be used for any kind of pixel grid manipulation (warping). For example the outputs of the commands below will respectively have larger pixels (new resolution being one quarter the original resolution), get shifted by 2.8 (by sub-pixel), get a shear of 2, and be tilted (projected). After running each, please open the output file and see the effect. @example $ astwarp flat-ir/xdf-f160w.fits --scale=0.25 $ astwarp flat-ir/xdf-f160w.fits --translate=2.8 $ astwarp flat-ir/xdf-f160w.fits --shear=2 $ astwarp flat-ir/xdf-f160w.fits --project=0.001,0.0005 @end example @noindent You can also combine multiple warps in one command. For example to first rotate the image, then scale it, run this command: @example $ astwarp flat-ir/xdf-f160w.fits --rotate=20 --scale=0.25 @end example If you have multiple warps, do them all in one command. Don't warp them in separate commands because the correlated noise will become too strong. As you see in the matrix that is printed when you run Warp, it merges all the warps into a single warping matrix (see @ref{Warping basics} and @ref{Merging multiple warpings}) and simply applies that just once. Recall that since this is done through matrix multiplication, order matters in the separate operations. In fact through Warp's @option{--matrix} option, you can directly request your desired final warp and don't have to break it up into different warps like above (see @ref{Invoking astwarp}). Fortunately these datasets are already aligned to the same pixel grid, so you don't actually need the files that were just generated. You can safely delete them all with the following command. Here, you see why we put the processed outputs that we need later into a separate directory. In this way, the top directory can be used for temporary files for testing that you can simply delete with a generic command like below. @example $ rm *.fits @end example @noindent To detect the objects in the image, we'll run NoiseChisel: @example $ mkdir noisechisel $ astnoisechisel flat-ir/xdf-f160w.fits -onoisechisel/xdf-f160w.fits @end example Read what NoiseChisel writes on the command-line. The curious thing you will notice is that while there were more than 3000 pseudo detections to find the pseudo-detection S/N, but there were only slightly more than 100 clumps to find the false clump S/N. We will see what caused this after a short review on the output of NoiseChisel. NoiseChisel's output is a single file containing multiple extensions. You can get basic information about the extensions in a FITS file with Gnuastro's Fits program (see @ref{Fits}) as shown below. It contains 6 extensions and the first (counted as zero) is blank (has no data). @example $ astfits noisechisel/xdf-f160w.fits @end example NoiseChisel puts some general information on its outputs in the FITS header of the respective extension. To see the full list of keywords, you can again use the Fits program like above, but also give it your desired extension/HDU. You can also give the extension number (as listed in the output above), for example @option{-h2} instead of @option{-hOBJECTS}. @example $ astfits noisechisel/xdf-f160w.fits -hOBJECTS @end example @cindex GNU Grep The @code{NUMLABS} keyword in NoiseChisel's @code{OBJECTS} extension contains the number of objects that was found by NoiseChisel in that run. Try to visually find it in the header keywords you saw above. To simplify the process, you can pipe the output of the command above into @code{grep} (a program for matching lines which is available on almost all Unix-like operating systems). @example $ astfits noisechisel/xdf-f160w.fits -hOBJECTS | grep NUMLABS @end example @cindex GNU Grep If you just want the value of the keyword and not the full FITS keyword line, you can use AWK. In the example below, AWK will print the third word (separated by white space characters) in any line that has a first column value of @code{NUMLABS}. You can also try this for the third HDU (called @code{CLUMPS}) to see the number of clumps. @example $ astfits noisechisel/xdf-f160w.fits -h2 \ | awk '$1=="NUMLABS" @{print $3@}' @end example Grep and AWK are simple, but very powerful command-line software for processing text files. Learning them properly can greatly simplify your processing, while improve your creativity, productivity and speed. When you get time, it is highly recommended to master them. The most common implementation of both is from GNU. Like almost all GNU software, both GNU Grep and GNU AWK have wonderful manuals which come with the program for free. You don't have to read the whole manual at once, they both start with great generic introductions to get you going fast. As described above, you can read both manuals or refresh your memory on your command-line with these commands: @example $ info awk $ info grep @end example @cindex GNOME You can now open NoiseChisel's output with SAO DS9 and visually inspect it. Just note that since there are multiple extensions, the easiest way to view the whole file is to open it as a ``Multi-extension data cube'' with the @option{-mecube} option as shown below. If you use GNOME (another GNU software, most common graphic user interface in GNU/Linux operating systems), please see @ref{Viewing multiextension FITS images} to open DS9 in multi-extension cube mode by default when using the GUI (double clicking on the file). @example $ ds9 -mecube noisechisel/xdf-f160w.fits -zscale -zoom to fit @end example Using Gnuastro's Fits program, you can also copy a HDU from one FITS file to another (for more, see @ref{HDU manipulation}). So if you want to have a FITS file with only the detected objects, you can run this command: @example $ astfits noisechisel/xdf-f160w.fits --copy=OBJECTS -oobjects.fits @end example One good way to see if you have missed any signal is to mask all the detected pixels and inspect the noise pixels. For this, you can use Gnuastro's Arithmetic program (in particular its @code{where} operator as shown below, see @ref{Arithmetic operators}). With this command, all input pixels that have a value larger than zero in the @code{OBJECTS} extension will be set to NaN in the output (written in @file{det-masked.fits}). If you change the @code{gt} (for ``greater than'') operator to @code{eq} (for ``equal''), all the un-detected (sky) pixels will be masked and you can see the detections. @example $ astarithmetic noisechisel/xdf-f160w.fits \ noisechisel/xdf-f160w.fits 0 gt nan where -h1 -h2 \ --output=nc-masked.fits @end example In some cases, you might want to use a different kernel with NoiseChisel (not the default one). To do that, you can use MakeProfiles (see @ref{MakeProfiles}) in the following manner to build a 2D Gaussian kernel with a FWHM of 3 pixels that extends 5 times the FWHM. This new kernel can later be fed into NoiseChisel with the @option{--kernel} option. @example $ astmkprof --kernel=gaussian,3,5 --oversample=1 -okernel-g-3-5.fits $ astnoisechisel flat-ir/xdf-f160w.fits --kernel=kernel-g-3-5.fits \ --output=nc-my-kernel.fits @end example NoiseChisel can produce ``Check images'' to help you visualize how each step is completed. You can see all the check images it can produce with this command. @example $ astnoisechisel --help | grep check @end example The check images are also multi-extension FITS files. After each check image is produced, open it with ds9 like NoiseChisel's output above and flip through the extensions to see each processing in detail. It is @emph{strongly} encouraged to play with the different parameters and use the respective check images to see which step is affected by your change. The three most useful check images are @option{--checkqthresh}, @option{--checkdetection}, and @option{--checksegmentation}. We can now get back to the curious situation we noticed after running NoiseChisel: the number of false clumps to find an S/N limit was very small (given the extent of this image). This is bad, because we use quantiles in NoiseChisel and such a small number will result in a relatively large scatter. Since this is a segmentation issue, let's see why this happens with @option{--checksegmentation}. @example $ astnoisechisel flat-ir/xdf-f160w.fits --checksegmentation @end example To help you get a result faster, when check images are requested, NoiseChisel doesn't finish its processing (unless you also call @option{--continueaftercheck}). NoiseChisel aborts with an explanation of why it stopped without finishing and the file name of the check image that it produced. The first five extensions are: the input image, the convolved image, the initially labeled detected regions, all the sky region (false) clumps, and those that will be used for S/N. The sky clumps are found over NoiseChisel's ``large tiles'' independently. When inspecting the fourth extension of the check image, it is interesting how NoiseChisel has ignored most large tiles and only used the few that we see, mostly on the edge. The reason that almost all internal large tiles are ignored is that galaxies are extended and this is a very deep (and small) image. Thanks to the PSF (see @ref{PSF}), no object will have a sharp truncation. We have not seen any abrupt break in the light profile of any galaxy: galaxies are always larger when we get deeper datasets. Therefore, in a noisy image, some light will always be left un-detected. To be less affected by this un-detected light, NoiseChisel has the @option{--minskyfrac} option (see @ref{General NoiseChisel options}): any tile that has a larger fraction of detected pixels will be ignored. So let's see what the default value of this option is (recall that with @option{-P}, you can list all the options with their values in Gnuastro's programs): @example $ astnoisechisel -P | grep minskyfrac @end example @noindent Try decreasing this value and re-running NoiseChisel to see the effect on the fraction of large tiles that will be used for finding false/sky clumps. Play a little with this parameter (give it different values and check the result). @example $ astnoisechisel flat-ir/xdf-f160w.fits --minskyfrac=0.5 \ --checksegmentation @end example The smaller the value to @option{--minskyfrac}, the more probable that un-detected light in the wings of galaxies will bias/affect the derived false clump S/N. So it is always important to find a good balance between a larger @option{--minskyfrac} while having a sufficient number of resulting clumps (to avoid scatter). NoiseChisel doesn't just find the labeled pixels, it also finds the Sky value and the Sky standard deviation in the final two extensions of its output. To generate a catalog of the colors, we will be using the NoiseChisel labeled image from the F160W image. But the Sky and Sky standard deviation values for each different filter will also be necessary. So we'll run NoiseChisel with our finalized parameters value on both filters (you can also put this option's value in a configuration file to avoid repeating it). @example $ astnoisechisel flat-ir/xdf-f105w.fits -onoisechisel/xdf-f105w.fits \ --minskyfrac=0.5 $ astnoisechisel flat-ir/xdf-f160w.fits -onoisechisel/xdf-f160w.fits \ --minskyfrac=0.5 @end example Now, we are ready to make a catalog. We want the object and clump labels from the F160W image. But the input, Sky and Sky standard deviation images should come from each filter. So, we'll run MakeCatalog on NoiseChisel's output differently for each filter. When making the F105W catalog, we'll use the @option{--objectsfile} and @option{--clumpsfile} options to tell MakeCatalog to read the object and clump labels from the F160W NoiseChisel output. When these options aren't given, MakeCatalog will look into the same input file for object and clump labels. For both filters, we'll ask for the ID, RA, Dec, Magnitude and signal-to-noise ratio (see @ref{Quantifying measurement limits}). To see a list of all the parameters that MakeCatalog can measure for you, run it with @option{--help} option. @example $ mkdir catalog $ astmkcatalog noisechisel/xdf-f160w.fits --zeropoint=25.94 \ --ids --ra --dec --magnitude --sn \ --output=catalog/xdf-f160w.fits $ astmkcatalog noisechisel/xdf-f105w.fits --zeropoint=26.27 \ --objectsfile=noisechisel/xdf-f160w.fits \ --clumpsfile=noisechisel/xdf-f160w.fits \ --ids --ra --dec --magnitude --sn \ --output=catalog/xdf-f105w.fits @end example MakeCatalog can also produce catalogs in plain text format. Please run the MakeCatalog commands above again and replace the @file{.fits} suffix, in the value to @option{--output}, with @file{.txt} (we will also be using the text file outputs later). When a clumps image is also given@footnote{MakeCatalog will look at the @code{WCLUMPS} keyword in the objects image to see if it should also use a clumps image or not.}, like this example, two catalogs will be made. If you asked for a plain text file output, two files will be made with the @file{_c.txt} and @file{_o.txt} suffixes. If MakeCatalog's output is requested to be FITS, the two catalogs will be in separate extensions of a single file. You can inspect the separate extensions with the Fits program like before (as shown below). Afterwards, you can inspect the table in each extension with Gnuastro's Table program (see @ref{Table}) as shown below. @example $ astfits catalog/xdf-f105w.fits # Extension information $ asttable catalog/xdf-f105w.fits -h1 --info # Objects catalog info. $ asttable catalog/xdf-f105w.fits -h1 # Objects catalog columns. $ asttable catalog/xdf-f105w.fits -h2 -i # Clumps catalog info. $ asttable catalog/xdf-f105w.fits -h2 # Clumps catalog columns. @end example As you see above, to see the column contents of each table, you can just remove the @option{--info} (or @option{-i}) option. If you want to print the contents of special column(s), just specify the column number(s) (counting from @code{1}, same as output of the command above) or the column name(s) (if they have one). For example, if you just want the objects and clumps magnitude and signal-to-noise ratio in the F160W filter. You can get it with the following commands. @example $ asttable catalog/xdf-f160w.fits -h1 -cMAGNITUDE -cSN $ asttable catalog/xdf-f160w.fits -h2 -cMAGNITUDE -cSN @end example The clumps catalog has two ID columns (one for the over-all clump ID and one for the ID of the clump in its host object), the magnitude column numbers differ between the object and clumps catalog. So if you want to specify the columns by number, you will need to change the numbers when viewing the clump and objects catalogs. This is a useful advantage of having/using column names. @example $ asttable catalog/xdf-f160w.fits -h1 -c4 -c5 $ asttable catalog/xdf-f160w.fits -h2 -c5 -c6 @end example Finally, the comments in MakeCatalog's output (in FITS headers or lines starting with @code{#} in plain text) contain some important information about the dataset that can be useful. Open @file{catalog/xdf-f160w_o.txt} in a text editor to see them. Since we used the same labeled image on both filters, the number of rows in both catalogs are the same. So, let's measure the colors of the objects in this image. We'll merge the two clump catalogs together into one using the @code{paste} program on the command-line. The output file will have each line of both catalogs merged into a single line. @example $ paste catalog/xdf-f160w_c.txt catalog/xdf-f105w_c.txt \ > xdf-f160w-f105w_c_p.txt @end example Open @file{xdf-f160w-f105w_c_p.txt} after making it to see how @command{paste} has operated. We can now use AWK to find the colors. We'll ask AWK to only use lines that don't start with @code{#} and don't have a NaN magnitude in the 9th column (F105W magnitude@footnote{Recall that the objects and clumps labels were made on the F160W image. On the F105W image, there might not be enough signal, so random scatter may give a negative total brightness and thus a NaN magnitude.}). We will also ignore columns which don't have reliable F105W magnitudes (with a S/N less than 7@footnote{The value of 7 is taken from the clump S/N threshold in F160W (where the clumps were defined).}). For the other lines, AWK will print the ID, positional columns and the difference between the respective magnitude columns. @example $ awk '!/^#/ && $11!="nan" && $12>7 @{print $1, $2, $3, $4, $11-$5@}' \ xdf-f160w-f105w_c_p.txt > catalog/xdf-f105w-f160w_c.txt @end example Gnuastro has a simple program for basic statistical analysis. The command below will print some basic information about the distribution (minimum, maximum, median and etc), along with a cute little ASCII histogram to visually help you understand the distribution on the command-line without the need for a graphic user interface (see @ref{Invoking aststatistics}). This ASCII histogram can be useful when you just want some coarse and general information on the input dataset. It is also useful when working on a server (where you may not have graphic user interface), and finally, its fast. @example $ aststatistics catalog/xdf-f105w-f160w_c.txt -c5 @end example You can later use Gnuastro's Statistics program with the @option{--histogram} option to build a much more fine-grained histogram as a table to feed into your favorite plotting program for a much more accurate/appealing plot. If you just want a specific measure, for example the mean, median and standard deviation, you can ask for them specifically: @example $ aststatistics catalog/xdf-f105w-f160w_c.txt -c5 --mean --median --std @end example Some researchers prefer to have colors in a fixed aperture for all the objects. The colors we calculated above used a different segmentation map for each object. This might not satisfy some science cases. To make a fixed aperture catalog, we should make a labeled image which has a fixed label for each aperture. That labeled image can be given to MakeCatalog instead of NoiseChisel's labeled detection image. @cindex GNU AWK We'll use the objects catalog in the F160W catalog we generated before for the positions and set the other parameters of each profile to be a fixed circle of radius 5 pixels (we want all apertures to be fixed after all). AWK is a wonderful tool for such jobs as the command below shows. @example $ awk '!/^#/@{print $1, $2, $3, 5, 5, 0, 0, 1, $1, 1@}' \ catalog/xdf-f160w_c.txt > catalog/apertures.txt @end example We can now feed this catalog into MakeProfiles to build the apertures for us. See @ref{Invoking astmkprof} for a description of the options. The most important for this particular job is @option{--mforflatpix}, it tells MakeProfiles that the values in the magnitude column should be used for each pixel of a flat profile. Without it, MakeProfiles would build the profiles such that the @emph{sum} of the pixels of each profile would have a @emph{magnitude} (in log-scale) of the value given in that column (what you would expect when simulating a galaxy for example). @example $ astmkprof catalog/apertures.txt --background=flat-ir/xdf-f160w.fits \ --clearcanvas --replace --type=int16 --mforflatpix \ --mode=wcs @end example The first thing you might notice in the printed information is that the profiles are not built in order. This is because MakeProfiles works in parallel and parallel CPU operations are asynchronous. Without @option{--replace}, the output is the same in any case. You can try running MakeProfiles with one thread (using @option{--numthreads=1} to see how order is respected in that case. Open the output @file{apertures.fits} file and see the result. Where the apertures overlap, you will notice that one label has replaced the other (because of the @option{--replace} option). In the future, MakeCatalog will be able to work with overlapping labels, but currently it doesn't. If you are interested, please join us in completing Gnuastro with added improvements like this (see task 14750 @footnote{@url{https://savannah.gnu.org/task/index.php?14750}}). @file{apertures.fits} labeled image can now be fed input into MakeCatalog. Similar to how we used the F160W labels for the F105W catalog: the labels don't have to be produced by NoiseChisel. In comparison with the previous MakeCatalog call, notice how 1) we have no more clumps image, 2) that we have set @option{--objectshdu=1} (since @file{apertures.fits} is not the output of NoiseChisel where the labeled image is in the third extension), and 3) that we are now using @option{--objid} instead of @option{--ids} to avoid warnings that some ID columns are only for clumps. @example $ astmkcatalog noisechisel/xdf-f105w.fits --zeropoint=26.27 \ --objectsfile=apertures.fits --objectshdu=1 \ --objid --ra --dec --magnitude --sn \ --output=catalog/xdf-f105w-aper.fits @end example Change the filter name and zeropoint magnitudes and run this command again to have the fixed aperture magnitude in the F160W filter also. From this point on, you can follow the previous steps to derive the color in a fixed aperture. We will now find some of the objects with the strongest color difference and make a cutout to inspect them visually: let's see what the objects with a color more than two magnitudes look like. @cindex AWK We'll use the @file{catalog/xdf-f105w-f160w_c.txt} file that we produced above. With the command below, all lines with a color value more than 2 will be put in @file{reddest.txt} and inspect it using @command{cat}. @example $ awk '$5>1' catalog/xdf-f105w-f160w_c.txt > reddest.txt $ cat reddest.txt @end example We can now feed @file{reddest.txt} into Gnuastro's crop to see what these objects look like. To keep things clean, we'll make a directory called @file{reddest} and ask Crop to save the crops in this directory. We'll also add a @file{-f160w.fits} suffix to the crops. @example $ mkdir crop $ astcrop --mode=wcs --coordcol=3 --coordcol=4 flat-ir/xdf-f160w.fits \ --catalog=reddest.txt --width=15/3600,15/3600 \ --suffix=-f160w.fits --output=crop @end example Like the MakeProfiles command above, you might notice that the crops aren't made in order. Since each crop is independent of the rest, the crops are done in parallel and parallel operations are asynchronous. In the command above, change @file{f160w} to @file{f105w} to make the crops in both filters. To view the crops more easily (not having to open ds9 for each image), you can convert the FITS crops into the JPEG format. @example $ for f in *.fits; do \ astconvertt $f --fluxlow=-0.001 --fluxhigh=0.005 --invert -ojpg; \ done @end example The loop above is in series: each file is processed only after the previous ones are complete. If you have @url{https://www.gnu.org/software/parallel, GNU Parallel}, you can greatly speed up this conversion. GNU Parallel will run the separate commands simultaneously on different CPU threads in parallel. For more information on efficiently using your threads, see @ref{Multi-threaded operations}. @example $ parallel astconvertt --fluxlow=-0.001 --fluxhigh=0.005 --invert \ -ojpg ::: *.fits @end example You can now easily use your general GUI image viewer to flip through the images more easily. On GNOME, you can use the ``Eye of GNOME'' image viewer (with executable name of @file{eog}). Run the command below and by pressing the @key{} key, you can flip through the images and compare them visually more easily. Of course, the flux ranges have been chosen generically here for seeing the fainter parts. Therefore, brighter objects will be fully black. @example $ eog 1-f105w.jpg @end example Another thing that is commonly needed is to visually mark these objects on the image. DS9 has ``Region''s for this purpose. You just have to convert your catalog into a ``region file'' to feed into DS9. To do that, you can use AWK again as shown below. @example $ cd .. $ awk 'BEGIN@{print "# Region file format: DS9 version 4.1"; \ print "global color=green width=2"; \ print "fk5";@} \ @{printf "circle(%s,%s,1\")\n", $3, $4;@}' reddest.txt \ > reddest.reg @end example This region file can be loaded into DS9 with its @option{-regions} option as shown below (see above for the other options): @example $ ds9 -mecube noisechisel/xdf-f160w.fits -zscale -zoom to fit \ -regions load all reddest.reg @end example Finally, if this book or any of the programs in Gnuastro have been useful for your research, please cite the respective papers. All Gnuastro programs have a @option{--cite} option to help you cite the authors' work more easily. For example: @example $ astmkcatalog --cite @end example @node Installation, Common program behavior, Tutorials, Top @chapter Installation @c This link is put here because the `Quick start' section of the first @c chapter is not the most eye-catching part of the manual and some users @c were seen to follow this ``Installation'' chapter title in search of the @c tarball and fast instructions. @cindex Installation The latest released version of Gnuastro source code is always available at the following URL: @url{http://ftpmirror.gnu.org/gnuastro/gnuastro-latest.tar.gz} @noindent @ref{Quick start} describes the commands necessary to configure, build, and install Gnuastro on your system. This chapter will be useful in cases where the simple procedure above is not sufficient, for example your system lacks a mandatory/optional dependency (in other words, you can't pass the @command{$ ./configure} step), or you want greater customization, or you want to build and install Gnuastro from other random points in its history, or you want a higher level of control on the installation. Thus if you were happy with downloading the tarball and following @ref{Quick start}, then you can safely ignore this chapter and come back to it in the future if you need more customization. @ref{Dependencies} describes the mandatory, optional and bootstrapping dependencies of Gnuastro. Only the first group are required/mandatory when you are building Gnuastro using a tarball (see @ref{Release tarball}), they are very basic and low-level tools used in most astronomical software, so you might already have them installed, if not they are very easy to install as described for each. @ref{Downloading the source} discusses the two methods you can obtain the source code: as a tarball (a significant snapshot in Gnuastro's history), or the full history@footnote{@ref{Bootstrapping dependencies} are required if you clone the full history.}. The latter allows you to build Gnuastro at any random point in its history (for example to get bug fixes or new features that are not released as a tarball yet). The building and installation of Gnuastro is heavily customizable, to learn more about them, see @ref{Build and install}. This section is essentially a thorough explanation of the steps in @ref{Quick start}. It discusses ways you can influence the building and installation. If you encounter any problems in the installation process, it is probably already explained in @ref{Known issues}. In @ref{Other useful software} the installation and usage of some other free software that are not directly required by Gnuastro but might be useful in conjunction with it is discussed. @menu * Dependencies:: Necessary packages for Gnuastro. * Downloading the source:: Ways to download the source code. * Build and install:: Configure, build and install Gnuastro. @end menu @node Dependencies, Downloading the source, Installation, Installation @section Dependencies The dependencies needed to build and install Gnuastro are defined by the features you want and how you would like to obtain the source code (see @ref{Downloading the source}). A minimal set of dependencies are mandatory, if they are not present you cannot get passed the configuration step. Such mandatory dependencies are therefore very basic (low-level) tools which are easy to obtain, build and install, see @ref{Mandatory dependencies} for a full discussion. If you have the packages of @ref{Optional dependencies}, Gnuastro will have additional functionality (for example converting FITS images to JPEG or PDF). If you are installing from a tarball as explained in @ref{Quick start}, you can stop reading after this section. However, if you decided to use the version controlled source instead of the tarball (see @ref{Version controlled source}), an additional bootstrapping step is required before configuration and its dependencies are explained in @ref{Bootstrapping dependencies}. @menu * Mandatory dependencies:: Gnuastro will not install without these. * Optional dependencies:: Adding more functionality. * Bootstrapping dependencies:: If you have the version controlled source. @end menu @node Mandatory dependencies, Optional dependencies, Dependencies, Dependencies @subsection Mandatory dependencies @cindex Dependencies, Gnuastro @cindex GNU build system The mandatory Gnuastro dependencies are very basic and low-level tools. They all follow the same basic GNU based build system (like that shown in @ref{Quick start}), so even if you don't have them, installing them should be pretty straightforward. In this section we explain each program and any specific note that might be necessary in the installation. @cindex Building from source @cindex Compiling from source @cindex Source code building @cindex Source code compilation @cindex Package managers The most basic choice is to build the packages from source yourself, instead of relying on your distribution's package management system. While the latter choice is indeed possible, we recommend that you build these dependencies yourself as discussed below. We will send out notifications in the @command{info-gnuastro} mailing list, see @ref{Announcements} when we find out that these requirements are updated. @enumerate @item For each package, Gnuastro might preform better (or require) certain configuration options that your distribution's package managers didn't add for you. If present, these configuration options are explained during the installation of each in the sections below. When the proper configuration has not been set, the programs should complain and inform you. @item Your distribution's pre-built package might not be the most recent release. @item For the libraries, they might separate the binary file from the header files, see @ref{Known issues}. @item Like any other tool, the science you derive from Gnuastro's tools highly depend on these lower level dependencies, so generally it is much better to have a close connection with them. By reading their manuals, installing them and staying up to date with changes/bugs in them, your scientific results and understanding will also correspondingly improve. @end enumerate @menu * GNU Scientific Library:: Installing GSL. * CFITSIO:: C interface to the FITS standard. * WCSLIB:: C interface to the WCS standard of FITS. @end menu @node GNU Scientific Library, CFITSIO, Mandatory dependencies, Mandatory dependencies @subsubsection GNU Scientific library @cindex GNU Scientific Library The @url{http://www.gnu.org/software/gsl/, GNU Scientific Library}, or GSL, is a large collection of functions that are very useful in scientific applications, for example integration, random number generation, and Fast Fourier Transform among many others. To install GSL from source, you can run the following commands after you have downloaded @url{ftp://ftp.gnu.org/gnu/gsl/gsl-latest.tar.gz, @file{gsl-latest.tar.gz}}: @example $ tar xf gsl-latest.tar.gz $ cd gsl-X.X # Replace X.X with version number. $ ./configure $ make -j8 # Replace 8 with no. CPU threads. $ make check $ sudo make install @end example @node CFITSIO, WCSLIB, GNU Scientific Library, Mandatory dependencies @subsubsection CFITSIO @cindex CFITSIO @cindex FITS standard @url{http://heasarc.gsfc.nasa.gov/fitsio/, CFITSIO} is the closest you can get to the pixels in a FITS image while remaining faithful to the @url{http://fits.gsfc.nasa.gov/fits_standard.html, FITS standard}. It is written by William Pence, the principal author of the FITS standard@footnote{Pence, W.D. et al. Definition of the Flexible Image Transport System (FITS), version 3.0. (2010) Astronomy and Astrophysics, Volume 524, id.A42, 40 pp.}, and is regularly updated. Setting the definitions for all other software packages using FITS images. @vindex --enable-reentrant @cindex Reentrancy, multiple file opening @cindex Multiple file opening, reentrancy Some GNU/Linux distributions have CFITSIO in their package managers, if it is available and updated, you can use it. One problem that might occur is that CFITSIO might not be configured with the @option{--enable-reentrant} option by the distribution. This option allows CFITSIO to open a file in multiple threads, it can thus provide great speed improvements. If CFITSIO was not configured with this option, any program which needs this capability will warn you and abort when you ask for multiple threads (see @ref{Multi-threaded operations}). To install CFITSIO from source, we strongly recommend that you have a look through Chapter 2 (Creating the CFITSIO library) of the CFITSIO manual and understand the options you can pass to @command{$ ./configure} (they aren't too much). This is a very basic package for most astronomical software and it is best that you configure it nicely with your system. Once you download the source and unpack it, the following configure script should be enough for most purposes. Don't forget to read chapter two of the manual though, for example the second option is only for 64bit systems. The manual also explains how to check if it has been installed correctly. CFITSIO comes with two executables called fpack and funpack. From their manual: they ``are standalone programs for compressing and uncompressing images and tables that are stored in the FITS (Flexible Image Transport System) data format. They are analogous to the gzip and gunzip compression programs except that they are optimized for the types of astronomical images that are often stored in FITS format''. The commands below will compile and install them on your system along with CFITSIO. They are not essential for Gnuastro, since they are just wrappers for functions within CFITSIO, but they can come in handy. The @command{make utils} command is only available for versions above 3.39, it will build these executables along with several other test executables which are deleted before the installation (otherwise they will also be installed). The CFITSIO installation from source process is given below. Let's assume you have downloaded @url{http://heasarc.gsfc.nasa.gov/FTP/software/fitsio/c/cfitsio_latest.tar.gz, @file{cfitsio_latest.tar.gz}} and are in the same directory: @example $ tar xf cfitsio_latest.tar.gz $ cd cfitsio $ ./configure --prefix=/usr/local --enable-sse2 --enable-reentrant $ make $ make utils $ ./testprog > testprog.lis $ diff testprog.lis testprog.out # Should have no output $ cmp testprog.fit testprog.std # Should have no output $ rm cookbook fitscopy imcopy smem speed testprog $ sudo make install @end example @node WCSLIB, , CFITSIO, Mandatory dependencies @subsubsection WCSLIB @cindex WCS @cindex WCSLIB @cindex World Coordinate System @url{http://www.atnf.csiro.au/people/mcalabre/WCS/, WCSLIB} is written and maintained by one of the authors of the World Coordinate System (WCS) definition in the @url{http://fits.gsfc.nasa.gov/fits_standard.html, FITS standard}@footnote{Greisen E.W., Calabretta M.R. (2002) Representation of world coordinates in FITS. Astronomy and Astrophysics, 395, 1061-1075.}, Mark Calabretta. It might be already built and ready in your distribution's package management system. However, here the installation from source is explained, for the advantages of installation from source please see @ref{Mandatory dependencies}. To install WCSLIB you will need to have CFITSIO already installed, see @ref{CFITSIO}. @vindex --without-pgplot WCSLIB also has plotting capabilities which use PGPLOT (a plotting library for C). If you wan to use those capabilities in WCSLIB, @ref{PGPLOT} provides the PGPLOT installation instructions. However PGPLOT is old@footnote{As of early June 2016, its most recent version was uploaded in February 2001.}, so its installation is not easy, there are also many great modern WCS plotting tools (mostly in written in Python). Hence, if you will not be using those plotting functions in WCSLIB, you can configure it with the @option{--without-pgplot} option as shown below. Let's assume you have downloaded @url{ftp://ftp.atnf.csiro.au/pub/software/wcslib/wcslib.tar.bz2, @file{wcslib.tar.bz2}} and are in the same directory: @example $ tar xf wcslib.tar.bz2 $ cd wcslib-X.X # Replace X.X with version number $ ./configure --without-pgplot LIBS="-pthread -lm" --disable-fortran $ make $ make check $ sudo make install @end example @node Optional dependencies, Bootstrapping dependencies, Mandatory dependencies, Dependencies @subsection Optional dependencies The libraries listed here are only used for very specific applications, therefore if you don't want these operations, Gnuastro will be built and installed without them and you don't have to have the dependencies. @cindex GPL Ghostscript If the @command{./configure} script can't find these requirements, it will warn you in the end that they are not present and notify you of the operation(s) you can't do due to not having them. If the output you request from a program requires a missing library, that program is going to warn you and abort. In the case of executables like GPL GhostScript, if you install them at a later time, the program will run. This is because if required libraries are not present at build time, the executables cannot be built, but an executable is called by the built program at run time so if it becomes available, it will be used. If you do install an optional library later, you will have to rebuild Gnuastro and reinstall it for it to take effect. @table @asis @item GNU Libtool @cindex GNU Libtool Libtool is a program to simplify managing of the libraries to build an executable (a program). GNU Libtool has some added functionality compared to other implementations. If GNU Libtool isn't present on your system at configuration time a warning will be printed and @ref{BuildProgram} won't be built or installed. The configure script will look into your search path (@code{PATH}) for GNU Libtool through the following executable names: @command{libtool} (acceptable only if it is the GNU implementation) or @command{glibtool}. See @ref{Installation directory} for more on @code{PATH}. GNU Libtool (the binary/executable file) is a low-level program that is probably already present on your system, and if not, is available in your operating system package manager@footnote{Note that we want the binary/executable Libtool program which can be run on the command-line. In Debian-based operating systems which separate various parts of a package, you want want @code{libtool-bin}, the @code{libtool} package won't contain the executable program.}. If you want to install GNU Libtool's latest version from source, please visit its @url{https://www.gnu.org/software/libtool/, webpage}. Gnuastro's tarball is shipped with an internal implementation of GNU Libtool. Even if you have GNU Libtool, Gnuastro's internal implementation is used for the building and installation of Gnuastro. As a result, you can still build, install and use Gnuastro even if you don't have GNU Libtool installed on your system. However, this internal Libtool does not get installed. Therefore, after Gnuastro's installation, if you want to use @ref{BuildProgram} to compile and link your own C source code which uses the @ref{Gnuastro library}, you need to have GNU Libtool available on your system (independent of Gnuastro). See @ref{Review of library fundamentals} to learn more about libraries. @item libgit2 @cindex Git @cindex libgit2 @cindex Version control systems Git is one of the most common version control systems (see @ref{Version controlled source}). When @file{libgit2} is present, and Gnuastro's programs are run within a version controlled directory, outputs will contain the version number of the working directory's repository for future reproducibility. See the @command{COMMIT} keyword header in @ref{Output headers} for a discussion. @item libjpeg @pindex libjpeg @cindex JPEG format libjpeg is only used by ConvertType to read from and write to JPEG images. @url{http://www.ijg.org/, libjpeg} is a very basic library that provides tools to read and write JPEG images, most of the GNU/Linux graphic programs and libraries use it. Therefore you most probably already have it installed. @url{http://libjpeg-turbo.virtualgl.org/, libjpeg-turbo} is an alternative to libjpeg. It uses SIMD instructions for ARM based systems that significantly decreases the processing time of JPEG compression and decompression algorithms. @item GPL Ghostscript @cindex GPL Ghostscript GPL Ghostscript's executable (@command{gs}) is called used by ConvertType to compile a PDF file from a source PostScript file, see @ref{ConvertType}. Therefore its headers (and libraries) are not needed. With a very high probability you already have it in your GNU/Linux distribution. Unfortunately it does not follow the standard GNU build style so installing it is very hard. It is best to rely on your distribution's package managers for this. @end table @node Bootstrapping dependencies, , Optional dependencies, Dependencies @subsection Bootstrapping dependencies Bootstrapping is only necessary if you have decided to obtain the full version controlled history of Gnuastro, see @ref{Version controlled source} and @ref{Bootstrapping}. Using the version controlled source enables you to always be up to date with the most recent development work of Gnuastro (bug fixes, new functionalities, improved algorithms and etc). If you have downloaded a tarball (see @ref{Downloading the source}), then you can ignore this subsection. To successfully run the bootstrapping process, there are some additional dependencies to those discussed in the previous subsections. These are low level tools that are used by a large collection of Unix-like operating systems programs, therefore they are most probably already available in your system. If they are not already installed, you should be able to easily find them in any GNU/Linux distribution package management system (@command{apt-get}, @command{yum}, @command{pacman} and etc). The short names in parenthesis in @command{typewriter} font after the package name can be used to search for them in your package manager. For the GNU Portability Library, GNU Autoconf Archive and @TeX{} Live, it is recommended to use the instructions here, not your operating system's package manager. @table @asis @item GNU Portability Library (Gnulib) @cindex GNU C library @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) To ensure portability for a wider range of operating systems (those that don't include GNU C library, namely glibc), Gnuastro depends on the GNU portability library, or Gnulib. Gnulib keeps a copy of all the functions in glibc, implemented (as much as possible) to be portable to other operating systems. The @file{bootstrap} script can automatically clone Gnulib (as a @file{gnulib/} directory inside Gnuastro), however, as described in @ref{Bootstrapping} this is not recommended. The recommended way to bootstrap Gnuastro is to first clone Gnulib and the Autoconf archives (see below) into a local directory outside of Gnuastro. Let's call it @file{DEVDIR}@footnote{If you are not a developer in Gnulib or Autoconf archives, @file{DEVDIR} can be a directory that you don't backup. In this way the large number of files in these projects won't slow down your backup process or take bandwidth (if you backup to a remote server).} (which you can set to any directory). Currently in Gnuastro, both Gnulib and Autoconf archives have to be cloned in the same top directory@footnote{If you already have the Autoconf archives in a separate directory, or can't clone it in the same directory as Gnulib, or you have it with another directory name (not @file{autoconf-archive/}), you can follow this short step. Set @file{AUTOCONFARCHIVES} to your desired address. Then define a symbolic link in @file{DEVDIR} with the following command so Gnuastro's bootstrap script can find it:@*@command{$ ln -s $AUTOCONFARCHIVES $DEVDIR/autoconf-archive}.} like the case here@footnote{If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the git protocol. In that case use the following URL for the HTTP protocol instead (for Autoconf archives, replace the name): @command{http://git.sv.gnu.org/r/gnulib.git}}: @example $ DEVDIR=/home/yourname/Development $ cd $DEVDIR $ git clone git://git.sv.gnu.org/gnulib.git $ git clone git://git.sv.gnu.org/autoconf-archive.git @end example @noindent You now have the full version controlled source of these two repositories in separate directories. Both these packages are regularly updated, so every once in a while, you can run @command{$ git pull} within them to get any possible updates. @item GNU Automake (@command{automake}) @cindex GNU Automake GNU Automake will build the @file{Makefile.in} files in each sub-directory using the (hand-written) @file{Makefile.am} files. The @file{Makefile.in}s are subsequently used to generate the @file{Makefile}s when the user runs @command{./configure} before building. @item GNU Autoconf (@command{autoconf}) @cindex GNU Autoconf GNU Autoconf will build the @file{configure} script using the configurations we have defined (hand-written) in @file{configure.ac}. @item GNU Autoconf Archive @cindex GNU Autoconf Archive These are a large collection of tests that can be called to run at @command{./configure} time. See the explanation under GNU Portability Library above for instructions on obtaining it and keeping it up to date. @item GNU Libtool (@command{libtool}) @cindex GNU Libtool GNU Libtool is in charge of building all the libraries in Gnuastro. The libraries contain functions that are used by more than one program and are installed for use in other programs. They are thus put in a separate directory (@file{lib/}). @item GNU help2man (@command{help2man}) @cindex GNU help2man GNU help2man is used to convert the output of the @option{--help} option (@ref{--help}) to the traditional Man page (@ref{Man pages}). @item @LaTeX{} and some @TeX{} packages @cindex @LaTeX{} @cindex @TeX{} Live Some of the figures in this book are built by @LaTeX{} (using the PGF/TikZ package). The @LaTeX{} source for those figures is version controlled for easy maintenance not the actual figures. So the @file{./boostrap} script will run @LaTeX{} to build the figures. The best way to install @LaTeX{} and all the necessary packages is through @url{https://www.tug.org/texlive/, @TeX{} live} which is a package manager for @TeX{} related tools that is independent of any operating system. It is thus preferred to the @TeX{} Live versions distributed by your operating system. To install @TeX{} Live, go to the webpage and download the appropriate installer by following the ``download'' link. Note that by default the full package repository will be downloaded and installed (around 4 Giga Bytes) which can take @emph{very} long to download and to update later. However, most packages are not needed by everyone, it is easier, faster and better to install only the ``Basic scheme'' (consisting of only the most basic @TeX{} and @LaTeX{} packages, which is less than 200 Mega bytes)@footnote{You can also download the DVD iso file at a later time to keep as a backup for when you don't have internet connection if you need a package.}. After the installation, be sure to set the environment variables as suggested in the end of the outputs. Any time you confront (need) a package you don't have, simply install it with a command like below (similar to how you install software from your operating system's package manager)@footnote{After running @TeX{}, or @LaTeX{}, you might get a warning complaining about a @file{missingfile}. Run `@command{tlmgr info missingfile}' to see the package(s) containing that file which you can install.}. To install all the necessary @TeX{} packages for a successful Gnuastro bootstrap, run this command: @example $ su # tlmgr install epsf jknapltx caption biblatex biber iftex \ etoolbox logreq xstring xkeyval pgf ms \ xcolor pgfplots times rsfs pstools epspdf @end example @item ImageMagick (@command{imagemagick}) @cindex ImageMagick ImageMagick is a wonderful and robust program for image manipulation on the command-line. @file{bootsrap} uses it to convert the book images into the formats necessary for the various book formats. @end table @node Downloading the source, Build and install, Dependencies, Installation @section Downloading the source Gnuastro's source code can be downloaded in two ways. As a tarball, ready to be configured and installed on your system (as described in @ref{Quick start}), see @ref{Release tarball}. If you want official releases of stable versions this is the best, easiest and most common option. Alternatively, you can clone the version controlled history of Gnuastro, run one extra bootstrapping step and then follow the same steps as the tarball. This will give you access to all the most recent work that will be included in the next release along with the full project history. The process is thoroughly introduced in @ref{Version controlled source}. @menu * Release tarball:: Download a stable official release. * Version controlled source:: Get and use the version controlled source. @end menu @node Release tarball, Version controlled source, Downloading the source, Downloading the source @subsection Release tarball A release tarball (commonly compressed) is the most common way of obtaining free and open source software. A tarball is a snapshot of one particular moment in the Gnuastro development history along with all the necessary files to configure, build, and install Gnuastro easily (see @ref{Quick start}). It is very straightforward and needs the least set of dependencies (see @ref{Mandatory dependencies}). Gnuastro has tarballs for official stable releases and pre-releases for testing. See @ref{Version numbering} for more on the two types of releases and the formats of the version numbers. The URLs for each type of release are given below. @table @asis @item Official stable releases (@url{http://ftp.gnu.org/gnu/gnuastro}): This URL hosts the official stable releases of Gnuastro. Always use the most recent version (see @ref{Version numbering}). By clicking on the ``Last modified'' title of the second column, the files will be sorted by their date which you can also use to find the latest version. It is recommended to use a mirror to download these tarballs, please visit @url{http://ftpmirror.gnu.org/gnuastro/} and see below. @item Pre-release tar-balls (@url{http://alpha.gnu.org/gnu/gnuastro}): This URL contains unofficial pre-release versions of Gnuastro. The pre-release versions of Gnuastro here are for enthusiasts to try out before an official release. If there are problems, or bugs then the testers will inform the developers to fix before the next official release. See @ref{Version numbering} to understand how the version numbers here are formatted. If you want to remain even more up-to-date with the developing activities, please clone the version controlled source as described in @ref{Version controlled source}. @end table @cindex Gzip @cindex Lzip Gnuastro's official/stable tarball is released with two formats: Gzip (with suffix @file{.tar.gz}) and Lzip (with suffix @file{.tar.lz}). The pre-release tarballs (after version 0.3) are released only as an Lzip tarball. Gzip is a very well-known and widely used compression program created by GNU and available in most systems. However, Lzip provides a better compression ratio and more robust archival capacity. For example Gnuastro 0.3's tarball was 2.9MB and 4.3MB with Lzip and Gzip respectively, see the @url{http://www.nongnu.org/lzip/lzip.html, Lzip webpage} for more. Lzip might not be pre-installed in your operating system, if so, installing it from your operating system's package manager or from source is very easy and fast (it is a very small program). The GNU FTP server is mirrored (has backups) in various locations on the globe (@url{http://www.gnu.org/order/ftp.html}). You can use the closest mirror to your location for a more faster download. Note that only some mirrors keep track of the pre-release (alpha) tarballs. Also note that if you want to download immediately after and announcement (see @ref{Announcements}), the mirrors might need some time to synchronize with the main GNU FTP server. @node Version controlled source, , Release tarball, Downloading the source @subsection Version controlled source @cindex Git @cindex Version control The publicly distributed Gnuastro tar-ball (for example @file{gnuastro-X.X.tar.gz}) does not contain the revision history, it is only a snapshot of the source code at one significant instant of Gnuastro's history (specified by the version number, see @ref{Version numbering}), ready to be configured and built. To be able to develop successfully, the revision history of the code can be very useful to track when something was added or changed, also some updates that are not yet officially released might be in it. We use Git for the version control of Gnuastro. For those who are not familiar with it, we recommend the Pro Git@footnote{@url{https://progit.org/}} book. The whole book is publicly available for online reading and downloading and does a wonderful job at explaining the concepts and best practices. Let's assume you want to keep Gnuastro in the @file{TOPGNUASTRO} directory (can be any directory, change the value below). The full version controlled history of Gnuastro can be cloned in @file{TOPGNUASTRO/gnuastro} by running the following commands@footnote{If your internet connection is active, but Git complains about the network, it might be due to your network setup not recognizing the Git protocol. In that case use the following URL which uses the HTTP protocol instead: @command{http://git.sv.gnu.org/r/gnuastro.git}}: @example $ TOPGNUASTRO=/home/yourname/Research/projects/ $ cd $TOPGNUASTRO $ git clone git://git.sv.gnu.org/gnuastro.git @end example @noindent The @file{$TOPGNUASTRO/gnuastro} directory will contain hand-written (version controlled) source code for Gnuastro's programs, libraries, this book and the tests. All are divided into sub-directories with standard and very descriptive names. The version controlled files in the top cloned directory are either mainly in capital letters (for example @file{THANKS} and @file{README}) or mainly written in small-caps (for example @file{configure.ac} and @file{Makefile.am}). The former are non-programming, standard writing for human readers containing high-level information about the whole package. The latter are instructions to customize the GNU build system for Gnuastro. The cloned Gnuastro source cannot immediately be configured, compiled, or installed since it only contains hand-written files, not automatically generated or imported files which do all the hard work of the build process. See @ref{Bootstrapping} for the process of generating and importing those files (it is very easy!). Once you have bootstrapped Gnuastro, you can run the standard procedures (in @ref{Quick start}). Very soon after you have cloned it, Gnuastro's main @file{master} branch will be updated on the main repository (since the developers are actively working on Gnuastro), for the best practices in keeping your local history in sync with the main repository see @ref{Synchronizing}. @menu * Bootstrapping:: Adding all the automatically generated files. * Synchronizing:: Keep your local clone up to date. @end menu @node Bootstrapping, Synchronizing, Version controlled source, Version controlled source @subsubsection Bootstrapping @cindex Bootstrapping @cindex GNU Autoconf Archive @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) @cindex Automatically created build files @noindent The version controlled source code lacks the source files that we have not written or are automatically built. These automatically generated files are included in the distributed tar ball for each distribution (for example @file{gnuastro-X.X.tar.gz}, see @ref{Version numbering}) and make it easy to immediately configure, build, and install Gnuastro. However from the perspective of version control, they are just bloatware and sources of confusion (since they are not changed by Gnuastro developers). The process of automatically building and importing necessary files into the cloned directory is known as @emph{bootstrapping}. All the instructions for an automatic bootstrapping are available in @file{bootstrap} and configured using @file{bootstrap.conf}. @file{bootstrap} is the only file not written by Gnuastro developers but is under version control to enable simple bootstrapping immediately after cloning. It is maintained by the GNU Portability Library (Gnulib) and this file is an identical copy, so do not make any changes in this file since it will be replaced when Gnulib releases an update. Make all your changes in @file{bootstrap.conf}. The bootstrapping process has its own separate set of dependencies, the full list is given in @ref{Bootstrapping dependencies}. They are generally very low-level and used by a very large set of commonly used programs, so they are probably already installed on your system. The simplest way to bootstrap Gnuastro is to simply run the bootstrap script within your cloned Gnuastro directory as shown below. However, please read the next paragraph before doing so (see @ref{Version controlled source} for @file{TOPGNUASTRO}). @example $ cd TOPGNUASTRO/gnuastro $ ./bootstrap # Requires internet connection @end example Without any options, @file{bootstrap} will clone Gnulib within your cloned Gnuastro directory (@file{TOPGNUASTRO/gnuastro/gnulib}) and download the necessary Autoconf archives macros. So if you run bootstrap like this, you will need an internet connection every time you decide to bootstrap. Also, Gnulib is a large package and cloning it can be slow. It will also keep the full Gnulib repository within your Gnuastro repository, so if another one of your projects also needs Gnulib, and you insist on running bootstrap like this, you will have two copies. In case you regularly backup your important files, Gnulib will also slow down the backup process. Therefore while the simple invocation above can be used with no problem, it is not recommended. To do better, see the next paragraph. The recommended way to get these two packages is thoroughly discussed in @ref{Bootstrapping dependencies} (in short: clone them in the separate @file{DEVDIR/} directory). The following commands will take you into the cloned Gnuastro directory and run the @file{bootstrap} script, while telling it to copy some files (instead of making symbolic links, with the @option{--copy} option, this is not mandatory@footnote{The @option{--copy} option is recommended because some backup systems might do strange things with symbolic links.}) and where to look for Gnulib (with the @option{--gnulib-srcdir} option). Please note that the address given to @option{--gnulib-srcdir} has to be an absolute address (so don't use @file{~} or @file{../} for example). @example $ cd $TOPGNUASTRO/gnuastro $ ./bootstrap --copy --gnulib-srcdir=$DEVDIR/gnulib @end example @cindex GNU Texinfo @cindex GNU Libtool @cindex GNU Autoconf @cindex GNU Automake @cindex GNU C library @cindex GNU build system Since Gnulib and Autoconf archives are now available in your local directories, you don't need an internet connection every time you decide to remove all untracked files and redo the bootstrap (see box below). You can also use the same command on any other project that uses Gnulib. All the necessary GNU C library functions, Autoconf macros and Automake inputs are now available along with the book figures. The standard GNU build system (@ref{Quick start}) will do the rest of the job. @cartouche @noindent @strong{Undoing the bootstrap:} During the development, it might happen that you want to remove all the automatically generated and imported files. In other words, you might want to reverse the bootstrap process. Fortunately Git has a good program for this job: @command{git clean}. Run the following command and every file that is not version controlled will be removed. @example git clean -fxd @end example @noindent It is best to commit any recent change before running this command. You might have created new files since the last commit and if they haven't been committed, they will all be gone forever (using @command{rm}). To get a list of the non-version controlled files instead of deleting them, add the @option{n} option to @command{git clean}, so it becomes @option{-fxdn}. @end cartouche Besides the @file{bootstrap} and @file{bootstrap.conf}, the @file{bootstrapped/} directory and @file{README-hacking} file are also related to the bootstrapping process. The former hosts all the imported (bootstrapped) directories. Thus, in the version controlled source, it only contains a @file{REAME} file, but in the distributed tar-ball it also contains sub-directories filled with all bootstrapped files. @file{README-hacking} contains a summary of the bootstrapping process discussed in this section. It is a necessary reference when you haven't built this book yet. It is thus not distributed in the Gnuastro tarball. @node Synchronizing, , Bootstrapping, Version controlled source @subsubsection Synchronizing The bootstrapping script (see @ref{Bootstrapping}) is not regularly needed: you mainly need it after you have cloned Gnuastro (once) and whenever you want to re-import the files from Gnulib, or Autoconf archives@footnote{@url{https://savannah.gnu.org/task/index.php?13993} is defined for you to check if significant (for Gnuastro) updates are made in these repositories, since the last time you pulled from them.} (not too common). However, Gnuastro developers are constantly working on Gnuastro and are pushing their changes to the official repository. Therefore, your local Gnuastro clone will soon be out-dated. Gnuastro has two mailing lists dedicated to its developing activities (see @ref{Developing mailing lists}). Subscribing to them can help you decide when to synchronize with the official repository. To pull all the most recent work in Gnuastro, run the following command from the top Gnuastro directory: @example $ git pull && autoconf -f @end example @cindex GNU Autoconf @cindex Mailing list: info-gnuastro @cindex @code{info-gnuastro@@gnu.org} GNU Autoconf is part of the GNU build system and will update the @file{./configure} script based on the hand-written configurations (in @file{configure.ac}, which is version controlled in Gnuastro). The pulled changes might contain changes in the build system configurations. However, The most important reason for running this command is to generate a version number for your Gnuastro snapshot. This generated version number will include the commit information if you are building Gnuastro from any point in Gnuastro's history (see @ref{Version numbering}). Since the version number is included in nearly all outputs of the programs, this can help you later exactly reproduce an old result by checking out the exact point in Gnuastro's history that produced those results. Therefore, be sure to run `@file{autoconf -f}' after every synchronization. You can also run them separately: @example $ git pull $ autoconf -f @end example If you would like to see what has changed since you last synchronized your local clone, you can take the following steps instead of the simple command above (don't type anything after @code{#}): @example $ git checkout master # Confirm if you are on master. $ git fetch origin # Fetch all new commits from server. $ git log master..origin/master # See all the new commit messages. $ git merge origin/master # Update your master branch. $ autoconf -f # Update ./configure. @end example @noindent By default @command{git log} prints the most recent commit first, add the @option{--reverse} option to see the changes chronologically. To see exactly what has been changed in the source code along with the commit message, add a @option{-p} option to the @command{git log}. If you intend make changes in the code, have a look at @ref{Developing} to get started easily. Be sure to commit your changes in a separate branch (keep your @code{master} branch to follow the official repository) and re-run @command{autoconf -f} after the commit. If you intend to send your changes to us (see @ref{Contributing to Gnuastro}) for the benefit of the whole community. If you send your work to us, you can safely use your commit since it will be ultimately recorded in Gnuastro's official history. If not, please upload your separate branch to a public hosting service (for example GitLab, see @ref{Forking tutorial}) and link to it in your report, or run @command{make distcheck} and upload the output @file{gnuastro-X.X.X.XXXX.tar.gz} to a publicly accessible webpage so your results can be considered scientific (reproducible). @node Build and install, , Downloading the source, Installation @section Build and install This section is basically a longer explanation to the sequence of commands given in @ref{Quick start}. If you didn't have any problems during the @ref{Quick start} steps, you want to have all the programs of Gnuastro installed in your system, you don't want to change the executable names during or after installation, you have root access to install the programs in the default system wide directory, the Letter paper size of the print book is fine for you or as a summary you don't feel like going into the details when everything is working, you can safely skip this section. If you have any of the above problems or you want to understand the details for a better control over your build and install, read along. The dependencies which you will need prior to configuring, building and installing Gnuastro are explained in @ref{Dependencies}. The first three steps in @ref{Quick start} need no extra explanation, so we will skip them and start with an explanation of Gnuastro specific configuration options and a discussion on the installation directory in @ref{Configuring}, followed by some smaller subsections: @ref{Tests}, @ref{A4 print book}, and @ref{Known issues} which explains the solutions to known problems you might encounter in the installation steps and ways you can solve them. @menu * Configuring:: Configure Gnuastro * Tests:: Run tests to see if it is working. * A4 print book:: Customize the print book. * Known issues:: Issues you might encounter. @end menu @node Configuring, Tests, Build and install, Build and install @subsection Configuring @pindex ./configure @cindex Configuring The @command{$ ./configure} step is the most important step in the build and install process. All the required packages, libraries, headers and environment variables are checked in this step. The behaviors of make and make install can also be set through command line options to this command. @cindex Configure options @cindex Customizing installation @cindex Installation, customizing The configure script accepts various arguments and options which enable the final user to highly customize whatever she is building. The options to configure are generally very similar to normal program options explained in @ref{Arguments and options}. Similar to all GNU programs, you can get a full list of the options along with a short explanation by running @example $ ./configure --help @end example @noindent @cindex GNU Autoconf A complete explanation is also included in the @file{INSTALL} file. Note that this file was written by the authors of GNU Autoconf (which builds the @file{configure} script), therefore it is common for all programs which use the @command{$ ./configure} script for building and installing, not just Gnuastro. Here we only discuss cases where you don't have super-user access to the system and if you want to change the executable names. But before that, a review of the options to configure that are particular to Gnuastro are discussed. @menu * Gnuastro configure options:: Configure options particular to Gnuastro. * Installation directory:: Specify the directory to install. * Executable names:: Changing executable names. * Configure and build in RAM:: For minimal use of HDD or SSD, and clean source. @end menu @node Gnuastro configure options, Installation directory, Configuring, Configuring @subsubsection Gnuastro configure options @cindex @command{./configure} options @cindex Configure options particular to Gnuastro Most of the options to configure (which are to do with building) are similar for every program which uses this script. Here the options that are particular to Gnuastro are discussed. The next topics explain the usage of other configure options which can be applied to any program using the GNU build system (through the configure script). @vtable @option @item --enable-progname Only build and install @file{progname} along with any other program that is enabled in this fashion. @file{progname} is the name of the executable without the @file{ast}, for example @file{crop} for Crop (with the executable name of @file{astcrop}). If this option is called for any of the programs in Gnuastro, any program which is not explicitly enabled will not be built or installed. @item --disable-progname @itemx --enable-progname=no Do not build or install the program named @file{progname}. This is very similar to the @option{--enable-progname}, but will build and install all the other programs except this one. @item --enable-gnulibcheck @cindex GNU C library @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) Enable checks on the GNU Portability Library (Gnulib). Gnulib is used by Gnuastro to enable users of non-GNU based operating systems (that don't use GNU C library or glibc) to compile and use the advanced features that this library provides. We make extensive use of such functions. If you give this option to @command{$ ./configure}, when you run @command{$ make check}, first the functions in Gnulib will be tested, then the Gnuastro executables. If your operating system does not support glibc or has an older version of it and you have problems in the build process (@command{$ make}), you can give this flag to configure to see if the problem is caused by Gnulib not supporting your operating system or Gnuastro, see @ref{Known issues}. @item --disable-guide-message @itemx --enable-guide-message=no Do not print a guiding message during the GNU Build process of @ref{Quick start}. By default, after each step, a message is printed guiding the user what the next command should be. Therefore, after @command{./configure}, it will suggest running @command{make}. After @command{make}, it will suggest running @command{make check} and so on. If Gnuastro is configured with this option, for example @example $ ./configure --disable-guide-message @end example Then these messages will not be printed after any step (like most programs). For people who are not yet fully accustomed to this build system, these guidelines can be very useful and encouraging. However, if you find those messages annoying, use this option. @end vtable @cartouche @noindent @strong{Note:} If some programs are enabled and some are disabled, it is equivalent to simply enabling those that were enabled. Listing the disabled programs is redundant. @end cartouche The tests of some programs might depend on the outputs of the tests of other programs. For example MakeProfiles is one the first programs to be tested when you run @command{$ make check}. MakeProfiles' test outputs (FITS images) are inputs to many other programs (which in turn provide inputs for other programs). Therefore, if you don't install MakeProfiles for example, the tests for many the other programs will be skipped. To avoid this, in one run, you can install all the programs and run the tests but not install. If everything is working correctly, you can run configure again with only the programs you want. However, don't run the tests and directly install after building. @node Installation directory, Executable names, Gnuastro configure options, Configuring @subsubsection Installation directory @vindex --prefix @cindex Superuser, not possible @cindex Root access, not possible @cindex No access to super-user install @cindex Install with no super-user access One of the most commonly used options to @file{./configure} is @option{--prefix}, it is used to define the directory that will host all the installed files (or the ``prefix'' in their final absolute file name). For example, when you are using a server and you don't have administrator or root access. In this example scenario, if you don't use the @option{--prefix} option, you won't be able to install the built files and thus access them from anywhere without having to worry about where they are installed. However, once you prepare your startup file to look into the proper place (as discussed thoroughly below), you will be able to easily use this option and benefit from any software you want to install without having to ask the system administrators or install and use a different version of a software that is already installed on the server. The most basic way to run an executable is to explicitly write its full file name (including all the directory information) and run it. One example is running the configuration script with the @command{$ ./configure} command (see @ref{Quick start}). By giving a specific directory (the current directory or @file{./}), we are explicitly telling the shell to look in the current directory for an executable file named `@file{configure}'. Directly specifying the directory is thus useful for executables in the current (or nearby) directories. However, when the program (an executable file) is to be used a lot, specifying all those directories will become a significant burden. For example, the @file{ls} executable lists the contents in a given directory and it is (usually) installed in the @file{/usr/bin/} directory by the operating system maintainers. So each time you want to use it you would have to run the following command (which is very inconvenient, both in writing and in remembering the various directories). @example $ /usr/bin/ls @end example @cindex Shell variables @cindex Environment variables To address this problem, we have the @file{PATH} environment variable. To understand it better, we will start with a short introduction to the shell variables. Shell variable values are basically treated as strings of characters. For example, it doesn't matter if the value is a name (string of @emph{alphabetic} characters) or a number (string of @emph{numeric} characters). You can define a variable and a value for it by running @example $ myvariable1=a_test_value $ myvariable2="a test value" @end example @noindent As you see above, if the value contains white space characters, you have to put the whole value (including white space characters) in double quotes (@key{"}). You can see the value it represents by running @example $ echo $myvariable1 $ echo $myvariable2 @end example @noindent @cindex Environment @cindex Environment variables If a variable has no value or it wasn't defined, the last command will only print an empty line. A variable defined like this will be known as long as this shell or terminal is running. Other terminals will have no idea it existed. The main advantage of shell variables is that if they are exported@footnote{By running @command{$ export myvariable=a_test_value} instead of the simpler case in the text}, subsequent programs that are run within that shell can access their value. So by changing their value, you can change the ``environment'' of a program which uses them. The shell variables which are accessed by programs are therefore known as ``environment variables''@footnote{You can use shell variables for other actions too, for example to temporarily keep some names or run loops on some files.}. You can see the full list of exported variables that your shell recognizes by running: @example $ printenv @end example @cindex @file{HOME} @cindex @file{HOME/.local/} @cindex Environment variable, @code{HOME} @file{HOME} is one commonly used environment variable, it is any user's (the one that is logged in) top directory. Try finding it in the command above. It is used so often that the shell has a special expansion (alternative) for it: `@file{~}'. Whenever you see file names starting with the tilde sign, it actually represents the value to the @file{HOME} environment variable, so @file{~/doc} is the same as @file{$HOME/doc}. @vindex PATH @pindex ./configure @cindex Setting @code{PATH} @cindex Default executable search directory @cindex Search directory for executables Another one of the most commonly used environment variables is @file{PATH}, it is a list of directories to search for executable names. Its value is a list of directories (separated by a colon, or `@key{:}'). When the address of the executable is not explicitly given (like @file{./configure} above), the system will look for the executable in the directories specified by @file{PATH}. If you have a computer nearby, try running the following command to see which directories your system will look into when it is searching for executable (binary) files, one example is printed here (notice how @file{/usr/bin}, in the @file{ls} example above, is one of the directories in @command{PATH}): @example $ echo $PATH /usr/local/sbin:/usr/local/bin:/usr/bin @end example By default @file{PATH} usually contains system-wide directories, which are readable (but not writable) by all users, like the above example. Therefore if you don't have root (or administrator) access, you need to add another directory to @file{PATH} which you actually have write access to. The standard directory where you can keep installed files (not just executables) for your own user is the @file{~/.local/} directory. The names of hidden files start with a `@key{.}' (dot), so it will not show up in your common command-line listings, or on the graphical user interface. You can use any other directory, but this is the most recognized. The top installation directory will be used to keep all the package's components: programs (executables), libraries, include (header) files, shared data (like manuals), or configuration files (see @ref{Review of library fundamentals} for a thorough introduction to headers and linking). So it commonly has some of the following sub-directories for each class of installed components respectively: @file{bin/}, @file{lib/}, @file{include/} @file{man/}, @file{share/}, @file{etc/}. Since the @file{PATH} variable is only used for executables, you can add the @file{~/.local/bin} directory (which keeps the executables/programs or more generally, ``binary'' files) to @file{PATH} with the following command. As defined below, first the existing value of @file{PATH} is used, then your given directory is added to its end and the combined value is put back in @file{PATH} (run `@command{$ echo $PATH}' afterwards to check if it was added). @example $ PATH=$PATH:~/.local/bin @end example @cindex GNU Bash @cindex Startup scripts @cindex Scripts, startup Any executable that you installed in @file{~/.local/bin} will now be usable without having to remember and write its full address. However, as soon as you leave/close your current terminal session, this modified @file{PATH} variable will be forgotten. Adding the directories which contain executables to the @file{PATH} environment variable each time you start a terminal is also very inconvenient and prone to errors. Fortunately, there are standard `startup files' defined by your shell precisely for this (and other) purposes. There is a special startup file for every significant starting step: @table @asis @cindex GNU Bash @item @file{/etc/profile} and everything in @file{/etc/profile.d/} These startup scripts are called when your whole system starts (for example after you turn on your computer). Therefore you need administrator or root privileges to access or modify them. @item @file{~/.bash_profile} If you are using (GNU) Bash as your shell, the commands in this file are run once every time you log in to your account. @item @file{~/.bashrc} If you are using (GNU) Bash as your shell, the commands here will be run each time you start a terminal (for example, when you open your terminal emulator in the graphic user interface). @end table For security reasons, it is highly recommended to directly type in your @file{HOME} directory value by hand in startup files instead of using variables. So in the following, let's assume your user name is `@file{name}' (so @file{~} may be replaced with @file{/home/name}). To add @file{~/.local/bin} to your @file{PATH} automatically on any startup file, you have to ``export'' the new value of @command{PATH} in the startup file that is most relevant to you by adding this line: @example export PATH=$PATH:/home/name/.local/bin @end example @cindex GNU build system @cindex Install directory @cindex Directory, install Now that you know your system will look into @file{~/.local/bin} for executables, you can tell Gnuastro's configure script to install everything in the top @file{~/.local} directory using the @option{--prefix} option. When you subsequently run @command{$ make install}, all the install-able files will be put in their respective directory under @file{~/.local/} (the executables in @file{~/.local/bin}, the compiled library files in @file{~/.local/lib}, the library header files in @file{~/.local/include} and so on, to learn more about these different files, please see @ref{Review of library fundamentals}). Note that tilde (`@key{~}') expansion will not happen if you put a `@key{=}' between @option{--prefix} and @file{~/.local}@footnote{If you insist on using `@key{=}', you can use @option{--prefix=$HOME/.local}.}, so we have avoided the @key{=} character here which is optional in GNU-style options, see @ref{Options}. @example $ ./configure --prefix ~/.local @end example @cindex @file{MANPATH} @cindex @file{INFOPATH} @cindex @file{LD_LIBRARY_PATH} @cindex Library search directory @cindex Default library search directory You can install everything (including libraries like GSL, CFITSIO, or WCSLIB which are Gnuastro's mandatory dependencies, see @ref{Mandatory dependencies}) locally by configuring them as above. However, recall that @command{PATH} is only for executable files, not libraries and that libraries can also depend on other libraries. For example WCSLIB depends on CFITSIO and Gnuastro needs both. Therefore, when you installed a library in a non-recognized directory, you have to guide the program that depends on them to look into the necessary library and header file directories. To do that, you have to define the @command{LDFLAGS} and @command{CPPFLAGS} environment variables respectively. This can be done while calling @file{./configure} as shown below: @example $ ./configure LDFLAGS=-L/home/name/.local/lib \ CPPFLAGS=-I/home/name/.local/include \ --prefix ~/.local @end example It can be annoying/buggy to do this when configuring every software that depends on such libraries. Hence, you can define these two variables in the most relevant startup file (discussed above). The convention on using these variables doesn't include a colon to separate values (as @command{PATH}-like variables do), they use white space characters and each value is prefixed with a compiler option@footnote{These variables are ultimately used as options while building the programs, so every value has be an option name followed be a value as discussed in @ref{Options}.}: note the @option{-L} and @option{-I} above (see @ref{Options}), for @option{-I} see @ref{Headers}, and for @option{-L}, see @ref{Linking}. Therefore we have to keep the value in double quotation signs to keep the white space characters and adding the following two lines to the startup file of choice: @example export LDFLAGS="$LDFLAGS -L/home/name/.local/lib" export CPPFLAGS="$CPPFLAGS -I/home/name/.local/include" @end example @cindex Dynamic libraries Dynamic libraries are linked to the executable every time you run a program that depends on them (see @ref{Linking} to fully understand this important concept). Hence dynamic libraries also require a special path variable called @command{LD_LIBRARY_PATH} (same formatting as @command{PATH}). To use programs that depend on these libraries, you need to add @file{~/.local/lib} to your @command{LD_LIBRARY_PATH} environment variable by adding the following line to the relevant start-up file: @example export LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/home/name/.local/lib @end example If you also want to access the Info (see @ref{Info}) and man pages (see @ref{Man pages}) documentations add @file{~/.local/share/info} and @file{~/.local/share/man} to your @command{INFOPATH}@footnote{Info has the following convention: ``If the value of @command{INFOPATH} ends with a colon [or it isn't defined] ..., the initial list of directories is constructed by appending the build-time default to the value of @command{INFOPATH}.'' So when installing in a non-standard directory and if @command{INFOPATH} was not initially defined, add a colon to the end of @command{INFOPATH} as shown below, otherwise Info will not be able to find system-wide installed documentation:@*@command{echo 'export INFOPATH=$INFOPATH:/home/name/.local/share/info:' >> ~/.bashrc}@* Note that this is only an internal convention of Info, do not use it for other @command{*PATH} variables.} and @command{MANPATH} environment variables respectively. @cindex Search directory order @cindex Order in search directory A final note is that order matters in the directories that are searched for all the variables discussed above. In the examples above, the new directory was added after the system specified directories. So if the program, library or manuals are found in the system wide directories, the user directory is no longer searched. If you want to search your local installation first, put the new directory before the already existing list, like the example below. @example export LD_LIBRARY_PATH=/home/name/.local/lib:$LD_LIBRARY_PATH @end example @noindent This is good when a library, for example CFITSIO, is already present on the system, but the system-wide install wasn't configured with the correct configuration flags (see @ref{CFITSIO}), or you want to use a newer version and you don't have administrator or root access to update it on the whole system/server. If you update @file{LD_LIBRARY_PATH} by placing @file{~/.local/lib} first (like above), the linker will first find the CFITSIO you installed for yourself and link with it. It thus will never reach the system-wide installation. There are important security problems with using local installations first: all important system-wide executables and libraries (important executables like @command{ls} and @command{cp}, or libraries like the C library) can be replaced by non-secure versions with the same file names and put in the customized directory (@file{~/.local} in this example). So if you choose to search in your customized directory first, please @emph{be sure} to keep it clean from executables or libraries with the same names as important system programs or libraries. @cartouche @noindent @strong{Summary:} When you are using a server which doesn't give you administrator/root access AND you would like to give priority to your own built programs and libraries, not the version that is (possibly already) present on the server, add these lines to your startup file. See above for which startup file is best for your case and for a detailed explanation on each. Don't forget to replace `@file{/YOUR-HOME-DIR}' with your home directory (for example `@file{/home/your-id}'): @example export PATH="/YOUR-HOME-DIR/.local/bin:$PATH" export LDFLAGS="-L/YOUR-HOME-DIR/.local/lib $LDFLAGS" export MANPATH="/YOUR-HOME-DIR/.local/share/man/:$MANPATH" export CPPFLAGS="-I/YOUR-HOME-DIR/.local/include $CPPFLAGS" export INFOPATH="/YOUR-HOME-DIR/.local/share/info/:$INFOPATH" export LD_LIBRARY_PATH="/YOUR-HOME-DIR/.local/lib:$LD_LIBRARY_PATH" @end example @noindent Afterwards, you just need to add an extra @option{--prefix=/YOUR-HOME-DIR/.local} to the @file{./configure} command of the software that you intend to install. Everything else will be the same as a standard build and install, see @ref{Quick start}. @end cartouche @node Executable names, Configure and build in RAM, Installation directory, Configuring @subsubsection Executable names @cindex Executable names @cindex Names of executables At first sight, the names of the executables for each program might seem to be uncommonly long, for example @command{astnoisechisel} or @command{astcrop}. We could have chosen terse (and cryptic) names like most programs do. We chose this complete naming convention (something like the commands in @TeX{}) so you don't have to spend too much time remembering what the name of a specific program was. Such complete names also enable you to easily search for the programs. @cindex Shell auto-complete @cindex Auto-complete in the shell To facilitate typing the names in, we suggest using the shell auto-complete. With this facility you can find the executable you want very easily. It is very similar to file name completion in the shell. For example, simply by typing the letters below (where @key{[TAB]} stands for the Tab key on your keyboard) @example $ ast[TAB][TAB] @end example @noindent you will get the list of all the available executables that start with @command{ast} in your @command{PATH} environment variable directories. So, all the Gnuastro executables installed on your system will be listed. Typing the next letter for the specific program you want along with a Tab, will limit this list until you get to your desired program. @cindex Names, customize @cindex Customize executable names In case all of this does not convince you and you still want to type short names, some suggestions are given below. You should have in mind though, that if you are writing a shell script that you might want to pass on to others, it is best to use the standard name because other users might not have adopted the same customizations. The long names also serve as a form of documentation in such scripts. A similar reasoning can be given for option names in scripts: it is good practice to always use the long formats of the options in shell scripts, see @ref{Options}. @cindex Symbolic link The simplest solution is making a symbolic link to the actual executable. For example let's assume you want to type @file{ic} to run Crop instead of @file{astcrop}. Assuming you installed Gnuastro executables in @file{/usr/local/bin} (default) you can do this simply by running the following command as root: @example # ln -s /usr/local/bin/astcrop /usr/local/bin/ic @end example @noindent In case you update Gnuastro and a new version of Crop is installed, the default executable name is the same, so your custom symbolic link still works. @vindex --program-prefix @vindex --program-suffix @vindex --program-transform-name The installed executable names can also be set using options to @command{$ ./configure}, see @ref{Configuring}. GNU Autoconf (which configures Gnuastro for your particular system), allows the builder to change the name of programs with the three options @option{--program-prefix}, @option{--program-suffix} and @option{--program-transform-name}. The first two are for adding a fixed prefix or suffix to all the programs that will be installed. This will actually make all the names longer! You can use it to add versions of program names to the programs in order to simultaneously have two executable versions of a program. @cindex SED, stream editor @cindex Stream editor, SED The third configure option allows you to set the executable name at install time using the SED program. SED is a very useful `stream editor'. There are various resources on the internet to use it effectively. However, we should caution that using configure options will change the actual executable name of the installed program and on every re-install (an update for example), you have to also add this option to keep the old executable name updated. Also note that the documentation or configuration files do not change from their standard names either. @cindex Removing @file{ast} from executables For example, let's assume that typing @file{ast} on every invocation of every program is really annoying you! You can remove this prefix from all the executables at configure time by adding this option: @example $ ./configure --program-transform-name='s/ast/ /' @end example @node Configure and build in RAM, , Executable names, Configuring @subsubsection Configure and build in RAM @cindex File I/O @cindex Input/Output, file The configure and build process involves the creation, reading, and modification of a large number of files (input/output, or I/O). Therefore file I/O issues can directly affect the work of developers who need to configure and build Gnuastro numerous times. Some of these issues are listed below: @itemize @cindex HDD @cindex SSD @item I/O will cause wear and tear on both the HDDs (mechanical failures) and SSDs (decreasing the lifetime). @cindex Backup @item Having the built files mixed with the source files can greatly affect backing up (synchronization) of source files (since it involves the management of a large number of small files that are regularly changed. Backup software can of course be configured to ignore the built files and directories. However, since the built files are mixed with the source files and can have a large variety, this will require a high level of customization. @end itemize @cindex tmpfs file system @cindex file systems, tmpfs One solution to address both these problems is to use the @url{https://en.wikipedia.org/wiki/Tmpfs, tmpfs file system}. Any file in tmpfs is actually stored in the RAM (and possibly SAWP), not on HDDs or SSDs. The RAM is built for extensive and fast I/O. Therefore the large number of file I/Os associated with configuring and building will not harm the HDDs or SSDs. Due to the volatile nature of RAM, files in the tmpfs file-system will be permanently lost after a power-off. Since all configured and built files are derivative files (not files that have been directly written by hand) there is no problem in this and this feature can be considered as an automatic cleanup. @cindex Linux kernel @cindex GNU C library @cindex GNU build system The modern GNU C library (and thus the Linux kernel) define the @file{/dev/shm} directory for this purpose (POSIX shared memory). So using GNU Build System's ability to build in a separate directory (not necessarily in the source directory), we can configure and build the programs in @file{/dev/shm} to benefit from the RAM. To simplify the process, Gnuastro comes with a @file{tmpfs-config-make} script. This script will create a directory in the shared memory, and put a symbolic link to it (called @file{build}) in the top source directory (the backup/sync software therefore only needs to ignore this single link/file). The script will then internally change to that directory and configure and build (@command{make -kjN}, where @command{N} is the number of threads for a parallel build) Gnuastro in there. To benefit from this script, simply run the following command instead of @command{./configure} and @command{make}: @example $ ./tmpfs-config-make @end example @cindex GNU Emacs After this script is finished, you can `@command{cd build}' and run other Make commands (for example, `@command{make check}', `@command{make install}', or `@command{make pdf}') from there. In Emacs, the command to be run with the @command{M-x compile} command (by default: @command{make -k}) can be changed to `@command{cd build; make -kjN}', or `@command{make -C build -kjN}' (@command{N} is the number of threads; an integer @mymath{\geq1}). For subsequent builds (during development) the @command{M-x recompile} command will also do all the building in the RAM while you modify the clean, and backed-up source files and make minimal/efficient use of your non-volatile HDD or SSD. This script can be used in any software which is configured and built using the GNU Build System. Just copy it in the top source directory of that software and run it from there. The default number of threads and location of the shared memory (@file{/dev/shm}) are currently hard-coded within the script. If you need to change them, please open the script with a text editor and set their values manually. @node Tests, A4 print book, Configuring, Build and install @subsection Tests @cindex @command{make check} @cindex @file{mock.fits} @cindex Tests, running @cindex Checking tests After successfully building (compiling) the programs with the @command{$ make} command you can check the installation before installing. To run the tests, run @example $ make check @end example For every program some tests are designed to check some possible operations. Running the command above will run those tests and give you a final report. If everything is ok and you have built all the programs, all the tests should pass. In case any of the tests fail, please have a look at @ref{Known issues} and if that still doesn't fix your problem, look that the @file{./tests/test-suite.log} file to see if the source of the error is something particular to your system or more general. If you feel it is general, please contact us because it might be a bug. Note that the tests of some programs depend on the outputs of other program's tests, so if you have not installed them they might be skipped or fail. Prior to releasing every distribution all these tests are checked. If you have a reasonably modern terminal, the outputs of the successful tests will be colored green and the failed ones will be colored red. These scripts can also act as a good set of examples for you to see how the programs are run. All the tests are in the @file{tests/} directory. The tests for each program are shell scripts (ending with @file{.sh}) in a sub-directory of this directory with the same name as the program. See @ref{Test scripts} for more detailed information about these scripts in case you want to inspect them. @node A4 print book, Known issues, Tests, Build and install @subsection A4 print book @cindex A4 print book @cindex Modifying print book @cindex A4 paper size @cindex US letter paper size @cindex Paper size, A4 @cindex Paper size, US letter The default print version of this book is provided in the letter paper size. If you would like to have the print version of this book on paper and you are living in a country which uses A4, then you can rebuild the book. The great thing about the GNU build system is that the book source code which is in Texinfo is also distributed with the program source code, enabling you to do such customizations (hacking). @cindex GNU Texinfo In order to change the paper size, you will need to have GNU Texinfo installed. Open @file{doc/gnuastro.texi} with any text editor. This is the source file that created this book. In the first few lines you will see this line: @example @@c@@afourpaper @end example @noindent In Texinfo, a line is commented with @code{@@c}. Therefore, un-comment this line by deleting the first two characters such that it changes to: @example @@afourpaper @end example @noindent Save the file and close it. You can now run @example $ make pdf @end example @noindent and the new PDF book will be available in @file{SRCdir/doc/gnuastro.pdf}. By changing the @command{pdf} in @command{$ make pdf} to @command{ps} or @command{dvi} you can have the book in those formats. Note that you can do this for any book that is in Texinfo format, they might not have @code{@@afourpaper} line, so you can add it close to the top of the Texinfo source file. @node Known issues, , A4 print book, Build and install @subsection Known issues Depending on your operating system and the version of the compiler you are using, you might confront some known problems during the configuration (@command{$ ./configure}), compilation (@command{$ make}) and tests (@command{$ make check}). Here, their solutions are discussed. @itemize @cindex Configuration, not finding library @cindex Development packages @item @command{$ ./configure}: @emph{Configure complains about not finding a library even though you have installed it.} The possible solution is based on how you installed the package: @itemize @item From your distribution's package manager. Most probably this is because your distribution has separated the header files of a library from the library parts. Please also install the `development' packages for those libraries too. Just add a @file{-dev} or @file{-devel} to the end of the package name and re-run the package manager. This will not happen if you install the libraries from source. When installed from source, the headers are also installed. @item @cindex @command{LDFLAGS} From source. Then your linker is not looking where you installed the library. If you followed the instructions in this chapter, all the libraries will be installed in @file{/usr/local/lib}. So you have to tell your linker to look in this directory. To do so, add @command{LDFLAGS=-L/usr/local/lib} to the Gnuastro configure script. If you want to use the libraries for your other programming projects, then export this environment variable similar to the case for @file{LD_LIBRARY_PATH} explained below. @end itemize @item @vindex --enable-gnulibcheck @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) @command{$ make}: @emph{Complains about an unknown function on a non-GNU based operating system.} In this case, please run @command{$ ./configure} with the @option{--enable-gnulibcheck} option to see if the problem is from the GNU Portability Library (Gnulib) not supporting your system or if there is a problem in Gnuastro, see @ref{Gnuastro configure options}. If the problem is not in Gnulib and after all its tests you get the same complaint from @command{make}, then please contact us at @file{bug-gnuastro@@gnu.org}. The cause is probably that a function that we have used is not supported by your operating system and we didn't included it along with the source tar ball. If the function is available in Gnulib, it can be fixed immediately. @item @cindex @command{CPPFLAGS} @command{$ make}: @emph{Can't find the headers (.h files) of libraries installed from source.} Similar to the case for @file{LDFLAGS} (above), your compiler is not looking in the right place, add @command{CPPFLAGS=-I/usr/local/include} to @command{./configure} to re-configure Gnuastro, then re-run make. @cindex Tests, only one passes @cindex @file{LD_LIBRARY_PATH} @item @command{$ make check}: @emph{Only one @file{.sh} test passes, all the rest fail.} It is highly likely that your distribution doesn't look into the @file{/usr/local/lib} directory when searching for shared libraries. To make sure it is added to the list of directories, run the following command and restart your terminal: (you can ignore the @command{\} and extra space if you type it, it is only necessary if you copy and paste). See @ref{Installation directory} for more details. @example echo 'export LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/lib' \ >> ~/.bashrc @end example @cindex GPL Ghostscript @item @command{$ make check}: @emph{The tests relying on external programs (for example @file{fitstopdf.sh} fail.}) This is probably due to the fact that the version number of the external programs is too old for the tests we have preformed. Please update the program to a more recent version. For example to create a PDF image, you will need GPL Ghostscript, but older versions do not work, we have successfully tested it on version 9.15. Older versions might cause a failure in the test result. @item @cindex @TeX{} @cindex GNU Texinfo @command{$ make pdf}: @emph{The PDF book cannot be made.} To make a PDF book, you need to have the GNU Texinfo program (like any program, the more recent the better). A working @TeX{} program is also necessary, which you can get from Tex Live@footnote{@url{https://www.tug.org/texlive/}}. @item @cindex GNU Libtool After @code{make check}: do not copy the programs' executables to another (for example, the installation) directory manually (using @command{cp}, or @command{mv} for example). In the default configuration@footnote{If you configure Gnuastro with the @option{--disable-shared} option, then the libraries will be statically linked to the programs and this problem won't exist, see @ref{Linking}.}, the program binaries need to link with Gnuastro's shared library which is also built and installed with the programs. Therefore, to run successfully before and after installation, linking modifications need to be made by GNU Libtool at installation time. @command{make install} does this internally, but a simple copy might give linking errors when you run it. If you need to copy the executables, you can do so after installation. @end itemize @noindent If your problem was not listed above, please file a bug report (@ref{Report a bug}). @node Common program behavior, Data containers, Installation, Top @chapter Common program behavior All the programs in Gnuastro share a set of common behavior mainly to do with user interaction to facilitate their usage. The most basic is how you can configure each program to do what you want: define the input, change parameter/option values, or identify the output. All Gnuastro programs can also read your desired configuration from pre-defined or user-specified files so you don't have to specify all the (sometimes numerous) parameters on the command-line each time you run a program. These files define the ``default'' program behavior in each directory, for each user, or on each system. In other cases, some programs can greatly benefit from the many threads available in modern CPUs, so here we'll also discuss how you can get the most out of your hardware. Among some other issues, we will also discuss how you can get immediate and distraction-free (without taking your hands off the keyboard!) help, or access to this whole book, on the command-line. @menu * Command-line:: How to use the command-line. * Configuration files:: Values for unspecified variables. * Multi-threaded operations:: How threads are managed in Gnuastro. * Numeric data types:: Different types and how to specify them. * Tables:: Recognized table formats. * Tessellation:: Tile the dataset into non-overlapping bins. * Getting help:: Getting more information on the go. * Automatic output:: About automatic output names. * Output headers:: Common headers to all FITS outputs. @end menu @node Command-line, Configuration files, Common program behavior, Common program behavior @section Command-line All the programs in Gnuastro are customized through the standard GNU style command-line options. Thus, we'll start by defining this general style that is very common in many command-line tools on Unix-like operating systems. Finally, the options that are common to all the programs in Gnuastro are discussed. @cindex Metacharacters @cindex Token separation @cindex Command-line token separation @cindex Separating tokens on the command-line The command-line text that you type is passed onto the shell (or program managing the command-line) as a string of characters. See the ``Invoking ProgramName'' sections in this manual for some examples of commands with each program, for example @ref{Invoking asttable}. That string is then broken up into separate @emph{tokens} or @emph{words} by any @emph{metacharacters} (like space, tab, @command{|}, @command{>} or @command{;}) that might exist in the text. To learn more, please see the GNU Bash manual, for the complete list of meta-characters and other GNU Bash definitions (GNU Bash is the most common shell program). Its ``Shell Operation'' section has a short summary of the steps the shell takes before passing the commands to the program you called. @menu * Arguments and options:: Basics of options and arguments. * Common options:: Common options to all Gnuastro programs. @end menu @node Arguments and options, Common options, Command-line, Command-line @subsection Arguments and options @cindex Options to programs @cindex Command-line options @cindex Arguments to programs @cindex Command-line arguments On the command-line, the first thing you usually enter is the name of the program you want to run. After that, you can specify two types of input: @emph{arguments} and @emph{options}. In the GNU-style, arguments are those tokens that are not preceded by any hyphens (@command{-}, see @ref{Arguments}). Here is one example: @example $ astcrop --center=53.162551,-27.789676 -w10/3600 --mode=wcs udf.fits @end example In this example, the argument is @file{udf.fits}. Arguments are most commonly the input file names containing your data. Options start with one or two hyphens, followed by an identifier for the option (the option's name) and its value (see @ref{Options}). Through options you tell the program how to interpret the data. In this example, we are running @ref{Crop} to crop a region of width 10 arc-seconds centered at the given RA and Dec from the input Hubble Ultra-Deep Field (UDF) FITS image. So options come with an identifier (the option name which is separate from their value). @vindex --help @vindex --usage @cindex Mandatory arguments Arguments can be both mandatory and optional and unlike options they don't have any identifiers (or help from you). Hence, their order might also matter (for example in @command{cp} which is used for copying one file to another location). The outputs of @option{--usage} and @option{--help} shows which arguments are optional and which are mandatory, see @ref{--usage}. As their name suggests, @emph{options} on the command-line can be considered to be optional and most of the time, you don't have to worry about what order you specify them in. When the order does matter, or the option can be invoked multiple times, it is explicitly mentioned in the ``Invoking ProgramName'' section of each program. @cindex Metacharacters on the command-line In case your arguments or option values contain any of the shell's meta-characters, you have to quote them. If there is only one such character, you can use a backslash (@command{\}) before it. If there are multiple, it might be easier to simply put your whole argument or option value inside of double quotes (@command{"}). In such cases, everything inside the double quotes will be seen as one token or word. @cindex HDU @cindex Header data unit For example, let's say you want to specify the header data unit (HDU) of your FITS file using a complex expression like `@command{3; images(exposure > 100)}'. If you simply add these after the @option{--hdu} (@option{-h}) option, the programs in Gnuastro will read the value to the HDU option as `@command{3}' and run. Then, Bash will attempt to run a separate command `@command{images(exposure > 100)}' and complain about a syntax error. This is because the semicolon (@command{;}) is an `end of command' character in the shell. To solve this problem you can simply put double quotes around the whole string you want to pass to @option{--hdu} as seen below: @example $ astcrop --hdu="3; images(exposure > 100)" FITSimage.fits @end example Alternatively you can put a `@command{\}' before every meta-character in this string, but try doing that, and probably you will agree that the double quotes are much more easier, elegant and readable. @menu * Arguments:: For specifying the main input files/operations. * Options:: For configuring the behavior of the program. @end menu @node Arguments, Options, Arguments and options, Arguments and options @subsubsection Arguments In Gnuastro, arguments are almost exclusively used as the input data file names. Please consult the first few paragraph of the ``Invoking ProgramName'' section for each program for a description of what it expects as input, how many arguments, or input data, it accepts, or in what order. Everything particular about how a program treats arguments, is explained under the ``Invoking ProgramName'' section for that program. Generally, if there is a standard file name extension for a particular format, that filename extension is used to separate the kinds of arguments. The list below shows the data formats that are recognized in Gnuastro's programs based on their file name endings. Any argument that doesn't end with the specified extensions below is considered to be a text file (usually catalogs, see @ref{Tables}). In some cases, a program can accept specific formats, for example @ref{ConvertType} also accepts @file{.jpg} images. @cindex Astronomical data suffixes @cindex Suffixes, astronomical data @itemize @item @file{.fits}: The standard file name ending of a FITS image. @item @file{.fit}: Alternative (3 character) FITS suffix. @item @file{.fits.Z}: A FITS image compressed with @command{compress}. @item @file{.fits.gz}: A FITS image compressed with GNU zip (gzip). @item @file{.fits.fz}: A FITS image compressed with @command{fpack}. @item @file{.imh}: IRAF format image file. @end itemize Through out this book and in the command-line outputs, whenever we want to generalize all such astronomical data formats in a text place holder, we will use @file{ASTRdata}, we will assume that the extension is also part of this name. Any file ending with these names is directly passed on to CFITSIO to read. Therefore you don't necessarily have to have these files on your computer, they can also be located on an FTP or HTTP server too, see the CFITSIO manual for more information. CFITSIO has its own error reporting techniques, if your input file(s) cannot be opened, or read, those errors will be printed prior to the final error by Gnuastro. @node Options, , Arguments, Arguments and options @subsubsection Options @cindex GNU style options @cindex Options, GNU style @cindex Options, short (@option{-}) and long (@option{--}) Command-line options allow configuring the behavior of a program in all GNU/Linux applications for each particular execution on a particular input data. A single option can be called in two ways: @emph{long} or @emph{short}. All options in Gnuastro accept the long format which has two hyphens an can have many characters (for example @option{--hdu}). Short options only have one hyphen (@key{-}) followed by one character (for example @option{-h}). You can see some examples in the list of options in @ref{Common options} or those for each program's ``Invoking ProgramName'' section. Both formats are shown for those which support both. First the short is shown then the long. Usually, the short options are for when you are writing on the command-line and want to save keystrokes and time. The long options are good for shell scripts, where you aren't usually rushing. Long options provide a level of documentation, since they are more descriptive and less cryptic. Usually after a few months of not running a program, the short options will be forgotten and reading your previously written script will not be easy. @cindex On/Off options @cindex Options, on/off Some options need to be given a value if they are called and some don't. You can think of the latter type of options as on/off options. These two types of options can be distinguished using the output of the @option{--help} and @option{--usage} options, which are common to all GNU software, see @ref{Getting help}. In Gnuastro we use the following strings to specify when the option needs a value and what format that value should be in. More specific tests will be done in the program and if the values are out of range (for example negative when the program only wants a positive value), an error will be reported. @vtable @option @item INT The value is read as an integer. @item FLT The value is read as a float. There are generally two types, depending on the context. If they are for fractions, they will have to be less than or equal to unity. @item STR The value is read as a string of characters (for example a file name) or other particular settings like a HDU name, see below. @end vtable @noindent @cindex Values to options @cindex Option values To specify a value in the short format, simply put the value after the option. Note that since the short options are only one character long, you don't have to type anything between the option and its value. For the long option you either need white space or an @option{=} sign, for example @option{-h2}, @option{-h 2}, @option{--hdu 2} or @option{--hdu=2} are all equivalent. The short format of on/off options (those that don't need values) can be concatenated for example these two hypothetical sequences of options are equivalent: @option{-a -b -c4} and @option{-abc4}. As an example, consider the following command to run Crop: @example $ astcrop -Dr3 --wwidth 3 catalog.txt --deccol=4 ASTRdata @end example @noindent The @command{$} is the shell prompt, @command{astcrop} is the program name. There are two arguments (@command{catalog.txt} and @command{ASTRdata}) and four options, two of them given in short format (@option{-D}, @option{-r}) and two in long format (@option{--width} and @option{--deccol}). Three of them require a value and one (@option{-D}) is an on/off option. @vindex --printparams @cindex Options, abbreviation @cindex Long option abbreviation If an abbreviation is unique between all the options of a program, the long option names can be abbreviated. For example, instead of typing @option{--printparams}, typing @option{--print} or maybe even @option{--pri} will be enough, if there are conflicts, the program will warn you and show you the alternatives. Finally, if you want the argument parser to stop parsing arguments beyond a certain point, you can use two dashes: @option{--}. No text on the command-line beyond these two dashes will be parsed. @cindex Repeated options @cindex Options, repeated Gnuastro has two types of options with values, those that only take a single value are the most common type. If these options are repeated or called more than once on the command-line, the value of the last time it was called will be assigned to it. This is very useful when you are testing/experimenting. Let's say you want to make a small modification to one option value. You can simply type the option with a new value in the end of the command and see how the script works. If you are satisfied with the change, you can remove the original option for human readability. If the change wasn't satisfactory, you can remove the one you just added and not worry about forgetting the original value. Without this capability, you would have to memorize or save the original value somewhere else, run the command and then change the value again which is not at all convenient and is potentially cause lots of bugs. On the other hand, some options can be called multiple times in one run of a program and can thus take multiple values (for example see the @option{--column} option in @ref{Invoking asttable}. In these cases, the order of stored values is the same order that you specified on the command-line. @cindex Configuration files @cindex Default option values Gnuastro's programs don't keep any internal default values, so some options are mandatory and if they don't have a value, the program will complain and abort. Most programs have many such options and typing them by hand on every call is impractical. To facilitate the user experience, after parsing the command-line, Gnuastro's programs read special configuration files to get the necessary values for the options you haven't identified on the command-line. These configuration files are fully described in @ref{Configuration files}. @cartouche @noindent @cindex Tilde expansion as option values @strong{CAUTION:} In specifying a file address, if you want to use the shell's tilde expansion (@command{~}) to specify your home directory, leave at least one space between the option name and your value. For example use @command{-o ~/test}, @command{--output ~/test} or @command{--output= ~/test}. Calling them with @command{-o~/test} or @command{--output=~/test} will disable shell expansion. @end cartouche @cartouche @noindent @strong{CAUTION:} If you forget to specify a value for an option which requires one, and that option is the last one, Gnuastro will warn you. But if it is in the middle of the command, it will take the text of the next option or argument as the value which can cause undefined behavior. @end cartouche @cartouche @noindent @cindex Counting from zero. @strong{NOTE:} In some contexts Gnuastro's counting starts from 0 and in others 1. You can assume by default that counting starts from 1, if it starts from 0 for a special option, it will be explicitly mentioned. @end cartouche @node Common options, , Arguments and options, Command-line @subsection Common options @cindex Options common to all programs @cindex Gnuastro common options To facilitate the job of the users and developers, all the programs in Gnuastro share some basic command-line options for the options that are common to many of the programs. The full list is classified as @ref{Input output options}, @ref{Processing options}, and @ref{Operating mode options}. In some programs, some of the options are irrelevant, but still recognized (you won't get an unrecognized option error, but the value isn't used). Unless otherwise mentioned, these options are identical between all programs. @menu * Input output options:: Common input/output options. * Processing options:: Options for common processing steps. * Operating mode options:: Common operating mode options. @end menu @node Input output options, Processing options, Common options, Common options @subsubsection Input/Output options These options are to do with the input and outputs of the various programs. @vtable @option @cindex HDU @cindex Header data unit @item -h STR/INT @itemx --hdu=STR/INT The name or number of the desired Header Data Unit, or HDU, in the FITS image. A FITS file can store multiple HDUs or extensions, each with either an image or a table or nothing at all (only a header). Note that counting of the extensions starts from 0(zero), not 1(one). Counting from 0 is forced on us by CFITSIO which directly reads the value you give with this option (see @ref{CFITSIO}). When specifying the name, case is not important so @command{IMAGE}, @command{image} or @command{ImAgE} are equivalent. CFITSIO has many capabilities to help you find the extension you want, far beyond the simple extension number and name. See CFITSIO manual's ``HDU Location Specification'' section for a very complete explanation with several examples. A @code{#} is appended to the string you specify for the HDU@footnote{With the @code{#} character, CFITSIO will only read the desired HDU into your memory, not all the existing HDUs in the fits file.} and the result is put in square brackets and appended to the FITS file name before calling CFITSIO to read the contents of the HDU for all the programs in Gnuastro. @item -s STR @itemx --searchin=STR Where to match/search for columns when the column identifier wasn't a number, see @ref{Selecting table columns}. The acceptable values are @command{name}, @command{unit}, or @command{comment}. This option is only relevant for programs that take table columns as input. @item -I @itemx --ignorecase Ignore case while matching/searching column meta-data (in the field specified by the @option{--searchin}). The FITS standard suggests to treat the column names as case insensitive, which is strongly recommended here also but is not enforced. This option is only relevant for programs that take table columns as input. This option is not relevant to @ref{BuildProgram}, hence in that program the short option @option{-I} is used for include directories, not to ignore case. @item -o STR @itemx --output=STR The name of the output file or directory. With this option the automatic output names explained in @ref{Automatic output} are ignored. @item -T STR @itemx --type=STR The data type of the output depending on the program context. This option isn't applicable to some programs like @ref{Fits} and will be ignored by them. The different acceptable values to this option are fully described in @ref{Numeric data types}. @item -D @itemx --dontdelete By default, if the output file already exists, Gnuastro's programs will silently delete it and put their own outputs in its place. When this option is activated, if the output file already exists, the programs will not delete it, will warn you, and will abort. @item -K @itemx --keepinputdir In automatic output names, don't remove the directory information of the input file names. As explained in @ref{Automatic output}, if no output name is specified (with @option{--output}), then the output name will be made in the existing directory based on your input's file name (ignoring the directory of the input). If you call this option, the directory information of the input will be kept and the automatically generated output name will be in the same directory as the input (usually with a suffix added). Note that his is only relevant if you are running the program in a different directory than the input data. @item -t STR @itemx --tableformat=STR The output table's type. This option is only relevant when the output is a table and its format cannot be deduced from its filename. For example, if a name ending in @file{.fits} was given to @option{--output}, then the program knows you want a FITS table. But there are two types of FITS tables: FITS ASCII, and FITS binary. Thus, with this option, the program is able to identify which type you want. The currently recognized values to this option are: @table @command @item txt A plain text table with white-space characters between the columns (see @ref{Gnuastro text table format}). @item fits-ascii A FITS ASCII table (see @ref{Recognized table formats}). @item fits-binary A FITS binary table (see @ref{Recognized table formats}). @end table @end vtable @node Processing options, Operating mode options, Input output options, Common options @subsubsection Processing options Some processing steps are common to several programs, so they are defined as common options to all programs. Note that this class of common options is thus necessarily less common between all the programs than those described in @ref{Input output options}, or @ref{Operating mode options} options. Also, if they are irrelevant for a program, these options will not display in the @option{--help} output of the program. @table @option @item --minmapsize=INT The minimum size (in bytes) to store the contents of each main processing array of a program as a file (on the non-volatile HDD/SSD), not in RAM. This can be very useful for large datasets which can be very memory intensive such that your RAM will not be sufficient to keep/process them. A random filename is assigned to the array (in a @file{.gnuastro} directory within the running directory) which will keep the contents of the array as long as it is necessary. When this option has a value of @code{0} (zero), all arrays that use this option in a program will actually be in a file (not in RAM). When the value is @code{-1} (largest possible number in the unsigned integer types) these arrays will be definitely allocated in RAM. However, for complex programs like @ref{NoiseChisel}, it is recommended to not set it to @code{0}, but a value like @code{10000} so the many small arrays necessary during processing are stored in RAM and only larger ones are saved as a file. Please note that using a non-volatile file (in the HDD/SDD) instead of RAM can significantly increase the program's running time, especially on HDDs. So it is best to give this option large values by default. You can then decrease it for a specific program's invocation on a large input after you see memory issues arise (for example an error, or the program not aborting and fully consuming your memory). The random file will be deleted once it is no longer needed by the program. The @file{.gnuastro} directory will also be deleted if it has no other contents (you may also have configuration files in this directory, see @ref{Configuration files}). If you see randomly named files remaining in this directory, please send us a bug report so we address the problem, see @ref{Report a bug}. @item -Z INT[,INT[,...]] @itemx --tilesize=[,INT[,...]] The size of regular tiles for tessellation, see @ref{Tessellation}. For each dimension an integer length (in units of data-elements or pixels) is necessary. If the number of input dimensions is different from the number of values given to this option, the program will stop with an error. Values must be separated by commas (@key{,}) and can also be fractions (for example @code{4/2}). If they are fractions, the result must be an integer, otherwise an error will be printed. @item -M INT[,INT[,...]] @itemx --numchannels=INT[,INT[,...]] The number of channels for larger input tessellation, see @ref{Tessellation}. The number and types of acceptable values are similar to @option{--tilesize}. The only difference is that instead of length, the integers values given to this option represent the @emph{number} of channels, not their size. @item -F FLT @itemx --remainderfrac=FLT The fraction of remainder size along all dimensions to add to the first tile. See @ref{Tessellation} for a complete description. This option is only relevant if @option{--tilesize} is not exactly divisible by the input dataset's size in a dimension. If the remainder size is larger than this fraction (compared to @option{--tilesize}), then the remainder size will be added with one regular tile size and divided between two tiles at the start and end of the given dimension. @item --workoverch Ignore the channel borders for the high-level job of the given application. As a result, while the channel borders are respected in defining the small tiles (such that no tile will cross a channel border), the higher-level program operation will ignore them, see @ref{Tessellation}. @item --checktiles Make a FITS file with the same dimensions as the input but each pixel is replaced with the ID of the tile that it is associated with. Note that the tile IDs start from 0. See @ref{Tessellation} for more on Tiling an image in Gnuastro. @item --oneelempertile When showing the tile values (for example with @option{--checktiles}, or when the program's output is tessellated) only use one element for each tile. This can be useful when only the relative values given to each tile compared to the rest are important or need to be checked. Since the tiles usually have a large number of pixels within them the output will be much smaller, and so easier to read, write, store, or send. Note that when the full input size in any dimension is not exactly divisible by the given @option{--tilesize} in that dimension, the edge tile(s) will have different sizes (in units of the input's size), see @option{--remainderfrac}. But with this option, all displayed values are going to have the (same) size of one data-element. Hence, in such cases, the image proportions are going to be slightly different with this option. If your input image is not exactly divisible by the tile size and you want one value per tile for some higher-level processing, all is not lost though. You can see how many pixels were within each tile (for example to weight the values or discard some for later processing) with Gnuastro's Statistics (see @ref{Statistics}) as shown below. The output FITS file is going to have two extensions, one with the median calculated on each tile and one with the number of elements that each tile covers. You can then use the @code{where} operator in @ref{Arithmetic} to set the values of all tiles that don't have the regular area to a blank value. @example $ aststatistics --median --number --ontile input.fits \ --oneelempertile --output=o.fits $ REGULAR_AREA=1600 # Check second extension of `o.fits'. $ astarithmetic o.fits o.fits $REGULAR_AREA ne nan where \ -h1 -h2 @end example Note that if @file{input.fits} also has blank values, then the median on tiles with blank values will also be ignored with the command above (which is desirable). @item --inteponlyblank When values are to be interpolated, only change the values of the blank elements, keep the non-blank elements untouched. @item --interpnumngb=INT The number of nearby non-blank neighbors to use for interpolation. @end table @node Operating mode options, , Processing options, Common options @subsubsection Operating mode options Another group of options that are common to all the programs in Gnuastro are those to do with the general operation of the programs. The explanation for those that are not only limited to Gnuastro but are common to all GNU programs start with (GNU option). @vtable @option @item -- (GNU option) Stop parsing the command-line. This option can be useful in scripts or when using the shell history. Suppose you have a long list of options, and want to see if removing some of them (to read from configuration files, see @ref{Configuration files}) can give a better result. If the ones you want to remove are the last ones on the command-line, you don't have to delete them, you can just add @option{--} before them and if you don't get what you want, you can remove the @option{--} and get the same initial result. @item --usage (GNU option) Only print the options and arguments and abort. This is very useful for when you know the what the options do, and have just forgot their long/short identifiers, see @ref{--usage}. @item -? @itemx --help (GNU option) Print all options with an explanation and abort. Adding this option will print all the options in their short and long formats, also displaying which ones need a value if they are called (with an @option{=} after the long format followed by a string specifying the format, see @ref{Options}). A short explanation is also given for what the option is for. The program will quit immediately after the message is printed and will not do any form of processing, see @ref{--help}. @item -V @itemx --version (GNU option) Print a short message, showing the full name, version, copyright information and program authors and abort. On the first line, it will print the official name (not executable name) and version number of the program. Following this is a blank line and a copyright information. The program will not run. @item -q @itemx --quiet Don't report steps. All the programs in Gnuastro that have multiple major steps will report their steps for you to follow while they are operating. If you do not want to see these reports, you can call this option and only error/warning messages will be printed. If the steps are done very fast (depending on the properties of your input) disabling these reports will also decrease running time. @item --cite Print the Bib@TeX{} entry for Gnuastro and the particular program (if that program comes with a separate paper) and abort. Citations are vital for the continued work on Gnuastro. Gnuastro started and is continued based on separate research projects. So if you find any of the tools offered in Gnuastro to be useful in your research, please use the output of this command to cite the program and Gnuastro in your research paper. Thank you. Gnuastro is still new, there is no separate paper only devoted to Gnuastro yet. Therefore currently the paper to cite for Gnuastro is the paper for NoiseChisel which is the first published paper introducing Gnuastro to the astronomical community. Upon reaching a certain point, a paper completely devoted to Gnuastro will be published, see @ref{GNU Astronomy Utilities 1.0}. @item -P @itemx --printparams With this option, Gnuastro's programs will read your command-line options and all the configuration files. If there is no problem (like a missing parameter or a value in the wrong format or range) and immediately before actually running, the programs will print the full list of option names, values and descriptions, sorted and grouped by context and abort. They will also report the version number, the date they were configured on your system and the time they were reported. As an example, you can give your full command-line options and even the input and output file names and finally just add @option{-P} to check if all the parameters are finely set. If everything is ok, you can just run the same command (easily retrieved from the shell history, with the top arrow key) and simply remove the last two characters that showed this option. Since no program will actually start its processing when this option is called, the otherwise mandatory arguments for each program (for example input image or catalog files) are no longer required when you call this option. @item --config=STR Parse @option{STR} as a configuration file immediately when this option is confronted (see @ref{Configuration files}). The @option{--config} option can be called multiple times in one run of any Gnuastro program on the command-line or in the configuration files. In any case, it will be immediately read (before parsing the rest of the options on the command-line, or lines in a configuration file). Note that by definition, later options on the command-line still take precedence over those in these in any configuration file, including the file(s) given to this option. Also see @option{--lastconfig} and @option{--onlyversion} on how this option can be used for reproducible results. @item -S @itemx --setdirconf Update the current directory configuration file for the Gnuastro program and quit. The full set of command-line and configuration file options will be parsed and options with a value will be written in the current directory configuration file for this program (see @ref{Configuration files}). If the configuration file or its directory doesn't exist, it will be created. If a configuration file exists it will be replaced (after it, and all other configuration files have been read). In any case, the program will not run. This is the recommended method@footnote{Alternatively, you can use your favorite text editor.} to edit/set the configuration file for all future calls to Gnuastro's programs. It will internally check if your values are in the correct range and type and save them according to the configuration file format, see @ref{Configuration file format}. So if there are unreasonable values to some options, the program will notify you and abort before writing the final configuration file. When this option is called, the otherwise mandatory arguments, for example input image or catalog file(s), are no longer mandatory (since the program will not run). @item -U @itemx --setusrconf Update the user configuration file and quit (see @ref{Configuration files}). See explanation under @option{--setdirconf} for more details. @item --lastconfig This is the last configuration file that must be read. When this option is confronted in any stage of reading the options (on the command-line or in a configuration file), no other configuration file will be parsed, see @ref{Configuration file precedence} and @ref{Current directory and User wide}. Like all on/off options, on the command-line, this option doesn't take any values. But in a configuration file, it takes the values of @option{0} or @option{1}, see @ref{Configuration file format}. If it is present in a configuration file with a value of @option{0}, then all later occurrences of this option will be ignored. @item --onlyversion=STR Only run the program if Gnuastro's version is exactly equal to @option{STR} (see @ref{Version numbering}). Note that it is not compared as a number, but as a string of characters, so @option{0}, or @option{0.0} and @option{0.00} are different. If the running Gnuastro version is different, then this option will report an error and abort as soon as it is confronted on the command-line or in a configuration file. If the running Gnuastro version is the same as @option{STR}, then the program will run as if this option was not called. This is useful if you want your results to be exactly reproducible and not mistakenly run with an updated/newer or older version of the program. Besides internal algorithmic/behavior changes in programs, the existence of options or their names might change between versions (especially in these earlier versions of Gnuastro). Hence, when using this option (probably in a script or in a configuration file), be sure to call it before other options. The benefit is that, when the version differs, the other options won't be parsed and you, or your collaborators/users, won't get errors saying an option in your configuration doesn't exist in the running version of the program. Here is one example of how this option can be used in conjunction with the @option{--lastconfig} option. Let's assume that you were satisfied with the results of this command: @command{astnoisechisel image.fits --detquant=0.95} (along with various options set in various configuration files). You can save the state of NoiseChisel and reproduce that exact result on @file{image.fits} later by following these steps (the the extra spaces, and @key{\}, are only for easy readability, if you want to try it out, only one space between each token is enough). @example $ echo "onlyversion X.XX" > reproducible.conf $ echo "lastconfig 1" >> reproducible.conf $ astnoisechisel image.fits --detquant=0.95 -P \ >> reproducible.conf @end example @option{--onlyversion} was available from Gnuastro 0.0, so putting it immediately at the start of a configuration file will ensure that later, you (or others using different version) won't get a non-recognized option error in case an option was added/removed. @option{--lastconfig} will inform the installed NoiseChisel to not parse any other configuration files. This is done because we don't want the user's user-wide or system wide option values affecting our results. Finally, with the third command, which has a @option{-P} (short for @option{--printparams}), NoiseChisel will print all the option values visible to it (in all the configuration files) and the shell will append them to @file{reproduce.conf}. Hence, you don't have to worry about remembering the (possibly) different options in the different configuration files. Afterwards, if you run NoiseChisel as shown below (telling it to read this configuration file with the @file{--config} option). You can be sure that there will either be an error (for version mis-match) or it will produce exactly the same result that you got before. @example $ astnoisechisel --config=reproducible.conf @end example @item --log Some programs can generate extra information about their outputs in a log file. When this option is called in those programs, the log file will also be printed. If the program doesn't generate a log file, this option is ignored. @cindex CPU threads, set number @cindex Number of CPU threads to use @item -N INT @itemx --numthreads=INT Use @option{INT} CPU threads when running a Gnuastro program (see @ref{Multi-threaded operations}). If the value is zero (@code{0}), or this option is not given on the command-line or any configuration file, the value will be determined at run-time: the maximum number of threads available to the system when you run a Gnuastro program. Note that multi-threaded programming is only relevant to some programs. In others, this option will be ignored. @end vtable @node Configuration files, Multi-threaded operations, Command-line, Common program behavior @section Configuration files @cindex @file{etc} @cindex Configuration files @cindex Necessary parameters @cindex Default option values @cindex File system Hierarchy Standard Each program needs a certain number of parameters to run. Supplying all the necessary parameters each time you run the program is very frustrating and prone to errors. Therefore all the programs read the values for the necessary options you have not given in the command line from one of several plain text files (which you can view and edit with any text editor). These files are known as configuration files and are usually kept in a directory named @file{etc/} according to the file system hierarchy standard@footnote{@url{http://en.wikipedia.org/wiki/Filesystem_Hierarchy_Standard}}. @vindex --output @vindex --numthreads @cindex CPU threads, number @cindex Internal default value @cindex Number of CPU threads to use The thing to have in mind is that none of the programs in Gnuastro keep any internal default value. All the values must either be stored in one of the configuration files or explicitly called in the command-line. In case the necessary parameters are not given through any of these methods, the program will print a missing option error and abort. The only exception to this is @option{--numthreads}, whose default value is determined at run-time using the number of threads available to your system, see @ref{Multi-threaded operations}. Of course, you can still provide a default value for the number of threads at any of the levels below, but if you don't, the program will not abort. Also note that through automatic output name generation, the value to the @option{--output} option is also not mandatory on the command-line or in the configuration files for all programs which don't rely on that value as an input@footnote{One example of a program which uses the value given to @option{--output} as an input is ConvertType, this value specifies the type of the output through the value to @option{--output}, see @ref{Invoking astconvertt}.}, see @ref{Automatic output}. @menu * Configuration file format:: ASCII format of configuration file. * Configuration file precedence:: Precedence of configuration files. * Current directory and User wide:: Local and user configuration files. * System wide:: System wide configuration files. @end menu @node Configuration file format, Configuration file precedence, Configuration files, Configuration files @subsection Configuration file format @cindex Configuration file suffix The configuration files for each program have the standard program executable name with a `@file{.conf}' suffix. When you download the source code, you can find them in the same directory as the source code of each program, see @ref{Program source}. @cindex White space character @cindex Configuration file format Any line in the configuration file whose first non-white character is a @key{#} is considered to be a comment and is ignored. An empty line is also similarly ignored. The long name of the option should be used as an identifier. The parameter name and parameter value have to be separated by any number of `white-space' characters: space, tab or vertical tab. By default several space characters are used. If the value of an option has space characters (most commonly for the @option{hdu} option), then the full value can be enclosed in double quotation signs (@key{"}, similar to the example in @ref{Arguments and options}). If it is an option without a value in the @option{--help} output (on/off option, see @ref{Options}), then the value should be @option{1} if it is to be `on' and @option{0} otherwise. In each non-commented and non-blank line, any text after the first two words (option identifier and value) is ignored. If an option identifier is not recognized in the configuration file, the name of the file, the line number of the unrecognized option, and the unrecognized identifier name will be reported and the program will abort. If a parameter is repeated more more than once in the configuration files, accepts only one value, and is not set on the command-line, then only the first value will be used, the rest will be ignored. @cindex Writing configuration files @cindex Automatic configuration file writing @cindex Configuration files, writing You can build or edit any of the directories and the configuration files yourself using any text editor. However, it is recommended to use the @option{--setdirconf} and @option{--setusrconf} options to set default values for the current directory or this user, see @ref{Operating mode options}. With these options, the values you give will be checked before writing in the configuration file. They will also print a set of commented lines guiding the reader and will also classify the options based on their context and write them in their logical order to be more understandable. @node Configuration file precedence, Current directory and User wide, Configuration file format, Configuration files @subsection Configuration file precedence @cindex Configuration file precedence @cindex Configuration file directories @cindex Precedence, configuration files The option values in all the programs of Gnuastro will be filled in the following order. If an option only takes one value which is given in an earlier step, any value for that option in a later step will be ignored. Note that if the @option{lastconfig} option is specified in any step below, all later files will be ignored (see @ref{Operating mode options}). The basic idea behind setting this progressive state of checking for parameter values is that separate users of a computer or separate folders in a user's file system might need different values for some parameters. In each step, there can also be a configuration file containing the common options in all the programs: @file{gnuastro.conf} (see @ref{Common options}). If options specific to one program are specified in this file, there will be un-recognized option errors, or unexpected behavior if the option has different behavior in another program. On the other hand, there is no problem with @file{astprogname.conf} containing common options@footnote{As an example, the @option{--setdirconf} and @option{--setusrconf} options will also write the common options they have read in their produced @file{astprogname.conf}.}. @enumerate @item Command-line options, for a particular run of ProgramName. @item @file{.gnuastro/astprogname.conf} is parsed by ProgramName in the current directory. @item @file{.gnuastro/gnuastro.conf} is parsed by all Gnuastro programs in the current directory. @item @file{$HOME/.local/etc/astprogname.conf} is parsed by ProgramName in the user's home directory (see @ref{Current directory and User wide}). @item @file{$HOME/.local/etc/gnuastro.conf} is parsed by all Gnuastro programs in the user's home directory (see @ref{Current directory and User wide}). @item @file{prefix/etc/astprogname.conf} is parsed by ProgramName in the system-wide installation directory (see @ref{System wide} for @file{prefix}). @item @file{prefix/etc/gnuastro.conf} is parsed by all Gnuastro programs in the system-wide installation directory (see @ref{System wide} for @file{prefix}). @end enumerate @cartouche @noindent @strong{Manipulating the order:} You can manipulate this order or add new files with the following two options which are fully described in @ref{Operating mode options}: @table @option @item --config Allows you to define any file to be parsed as a configuration file on the command-line or within the any other configuration file. Recall that the file given to @option{--config} is parsed immediately when this option is confronted (on the command-line or in a configuration file). @item --lastconfig Allows you to stop the parsing of subsequent configuration files. Note that if this option is given in a configuration file, it will be fully read, so its position in the configuration doesn't matter (unlike @option{--config}). @end table @end cartouche One example of benefiting from these configuration files can be this: raw telescope images usually have their main image extension in the second FITS extension, while processed FITS images usually only have one extension. If your system-wide default input extension is 0 (the first), then when you want to work with the former group of data you have to explicitly mention it to the programs every time. With this progressive state of default values to check, you can set different default values for the different directories that you would like to run Gnuastro in for your different purposes, so you won't have to worry about this issue any more. The same can be said about the @file{gnuastro.conf} files: by specifying a behavior in this single file, all Gnuastro programs in the respective directory, user, or system-wide steps will behave similarly. For example to keep the input's directory when no specific output is given (see @ref{Automatic output}), or to not delete an existing file if it has the same name as a given output (see @ref{Input output options}). @node Current directory and User wide, System wide, Configuration file precedence, Configuration files @subsection Current directory and User wide @cindex @file{$HOME} @cindex @file{./.gnuastro/} @cindex @file{$HOME/.local/etc/} For the current (local) and user-wide directories, the configuration files are stored in the hidden sub-directories named @file{.gnuastro/} and @file{$HOME/.local/etc/} respectively. Unless you have changed it, the @file{$HOME} environment variable should point to your home directory. You can check it by running @command{$ echo $HOME}. Each time you run any of the programs in Gnuastro, this environment variable is read and placed in the above address. So if you suddenly see that your home configuration files are not being read, probably you (or some other program) has changed the value of this environment variable. @vindex --setdirconf @vindex --setusrconf Although it might cause confusions like above, this dependence on the @file{HOME} environment variable enables you to temporarily use a different directory as your home directory. This can come in handy in complicated situations. To set the user or current directory configuration files based on your command-line input, you can use the @option{--setdirconf} or @option{--setusrconf}, see @ref{Operating mode options}. @node System wide, , Current directory and User wide, Configuration files @subsection System wide @cindex @file{prefix/etc/} @cindex System wide configuration files @cindex Configuration files, system wide When Gnuastro is installed, the configuration files that are shipped with the distribution are copied into the (possibly system wide) @file{prefix/etc/} directory. For more details on @file{prefix}, see @ref{Installation directory} (by default it is: @file{/usr/local}). This directory is the final place (with the lowest priority) that the programs in Gnuastro will check to retrieve parameter values. If you remove an option and its value from the system wide configuration files, you either have to specify it in more immediate configuration files or set it each time in the command-line. Recall that none of the programs in Gnuastro keep any internal default values and will abort if they don't find a value for the necessary parameters (except the number of threads and output file name). So even though you might never expect to use an optional option, it safe to have it available in this system-wide configuration file even if you don't intend to use it frequently. Note that in case you install Gnuastro from your distribution's repositories, @file{prefix} will either be set to @file{/} (the root directory) or @file{/usr}, so you can find the system wide configuration variables in @file{/etc/} or @file{/usr/etc/}. The prefix of @file{/usr/local/} is conventionally used for programs you install from source by your self as in @ref{Quick start}. @node Multi-threaded operations, Numeric data types, Configuration files, Common program behavior @section Multi-threaded operations @pindex nproc @cindex pthread @cindex CPU threads @cindex GNU Coreutils @cindex Using CPU threads @cindex CPU, using all threads @cindex Multi-threaded programs @cindex Using multiple CPU cores @cindex Simultaneous multithreading Some of the programs benefit significantly when you use all the threads your computer's CPU has to offer to your operating system. The number of threads available can be larger than the number of physical (hardware) cores in the CPU (also known as Simultaneous multithreading). For example, in Intel's CPUs (those that implement its Hyper-threading technology) the number of threads is usually double the number of physical cores in your CPU. On a GNU/Linux system, the number of threads available can be found with the command @command{$ nproc} command (part of GNU Coreutils). @vindex --numthreads @cindex Number of threads available @cindex Available number of threads @cindex Internally stored option value Gnuastro's programs can find the number of threads available to your system internally at run-time (when you execute the program). However, if a value is given to the @option{--numthreads} option, the given number will be used, see @ref{Operating mode options} and @ref{Configuration files} for ways to use this option. Thus @option{--numthreads} is the only common option in Gnuastro's programs with a value that doesn't have to be specified anywhere on the command-line or in the configuration files. @menu * A note on threads:: Caution and suggestion on using threads. * How to run simultaneous operations:: How to run things simultaneously. @end menu @node A note on threads, How to run simultaneous operations, Multi-threaded operations, Multi-threaded operations @subsection A note on threads @cindex Using multiple threads @cindex Best use of CPU threads @cindex Efficient use of CPU threads Spinning off threads is not necessarily the most efficient way to run an application. Creating a new thread isn't a cheap operation for the operating system. It is most useful when the input data are fixed and you want the same operation to be done on parts of it. For example one input image to Crop and multiple crops from various parts of it. In this fashion, the image is loaded into memory once, all the crops are divided between the number of threads internally and each thread cuts out those parts which are assigned to it from the same image. On the other hand, if you have multiple images and you want to crop the same region(s) out of all of them, it is much more efficient to set @option{--numthreads=1} (so no threads spin off) and run Crop multiple times simultaneously, see @ref{How to run simultaneous operations}. @cindex Wall-clock time You can check the boost in speed by first running a program on one of the data sets with the maximum number of threads and another time (with everything else the same) and only using one thread. You will notice that the wall-clock time (reported by most programs at their end) in the former is longer than the latter divided by number of physical CPU cores (not threads) available to your operating system. Asymptotically these two times can be equal (most of the time they aren't). So limiting the programs to use only one thread and running them independently on the number of available threads will be more efficient. @cindex System Cache @cindex Cache, system Note that the operating system keeps a cache of recently processed data, so usually, the second time you process an identical data set (independent of the number of threads used), you will get faster results. In order to make an unbiased comparison, you have to first clean the system's cache with the following command between the two runs. @example $ sync; echo 3 | sudo tee /proc/sys/vm/drop_caches @end example @cartouche @noindent @strong{SUMMARY: Should I use multiple threads?} Depends: @itemize @item If you only have @strong{one} data set (image in most cases!), then yes, the more threads you use (with a maximum of the number of threads available to your OS) the faster you will get your results. @item If you want to run the same operation on @strong{multiple} data sets, it is best to set the number of threads to 1 and use Make, or GNU Parallel, as explained in @ref{How to run simultaneous operations}. @end itemize @end cartouche @node How to run simultaneous operations, , A note on threads, Multi-threaded operations @subsection How to run simultaneous operations There are two@footnote{A third way would be to open multiple terminal emulator windows in your GUI, type the commands separately on each and press @key{Enter} once on each terminal, but this is far too frustrating, tedious and prone to errors. It's therefore not a realistic solution when tens, hundreds or thousands of operations (your research targets, multiplied by the operations you do on each) are to be done.} approaches to simultaneously execute a program: using GNU Parallel or Make (GNU Make is the most common implementation). The first is very useful when you only want to do one job multiple times and want to get back to your work without actually keeping the command you ran. The second is usually for more important operations, with lots of dependencies between the different products (for example a full scientific research). @table @asis @item GNU Parallel @cindex GNU Parallel When you only want to run multiple instances of a command on different threads and get on with the rest of your work, the best method is to use GNU parallel. Surprisingly GNU Parallel is one of the few GNU packages that has no Info documentation but only a Man page, see @ref{Info}. So to see the documentation after installing it please run @example $ man parallel @end example @noindent As an example, let's assume we want to crop a region fixed on the pixels (500, 600) with the default width from all the FITS images in the @file{./data} directory ending with @file{sci.fits} to the current directory. To do this, you can run: @example $ parallel astcrop --numthreads=1 --xc=500 --yc=600 ::: \ ./data/*sci.fits @end example @noindent GNU Parallel can help in many more conditions, this is one of the simplest, see the man page for lots of other examples. For absolute beginners: the backslash (@command{\}) is only a line breaker to fit nicely in the page. If you type the whole command in one line, you should remove it. @item Make @cindex Make Make is a program for building ``targets'' (e.g., files) using ``recipes'' (a set of operations) when their known ``prerequisites'' (other files) have been updated. It elegantly allows you to define dependency structures for building your final output and updating it efficiently when the inputs change. It is the most common infra-structure to build software today. Scientific research methodology is very similar to software development: you start by testing a hypothesis on a small sample of objects/targets with a simple set of steps. As you are able to get promising results, you improve the method and use it on a larger, more general, sample. In the process, you will confront many issues that have to be corrected (bugs in software development jargon). Make a wonderful tool to manage this style of development. It has been used to make reproducible papers, for example see @url{https://gitlab.com/makhlaghi/NoiseChisel-paper, the reproduction pipeline} of the paper introducing @ref{NoiseChisel} (one of Gnuastro's programs). @cindex GNU Make GNU Make@footnote{@url{https://www.gnu.org/software/make/}} is the most common implementation which (similar to nearly all GNU programs, comes with a wonderful manual@footnote{@url{https://www.gnu.org/software/make/manual/}}). Make is very basic and simple, and thus the manual is short (the most important parts are in the first roughly 100 pages) and easy to read/understand. Make comes with a @option{--jobs} (@option{-j}) option which allows you to specify the maximum number of jobs that can be done simultaneously. For example if you have 8 threads available to your operating system. You can run: @example $ make -j8 @end example With this command, Make will process your @file{Makefile} and create all the targets (can be thousands of FITS images for example) simultaneously on 8 threads, while fully respecting their dependencies (only building a file/target when its prerequisites are successfully built). Make is thus strongly recommended for managing scientific research where robustness, archivability, reproducibility and speed@footnote{Besides its multi-threaded capabilities, Make will only re-build those targets that depend on a change you have made, not the whole work. For example, if you have set the prerequisites properly, you can easily test the changing of a parameter on your paper's results without having to re-do everything (which is much faster). This allows you to be much more productive in easily checking various ideas/assumptions of the different stages of your research and thus produce a more robust result for your exciting science.} are very important. @end table @node Numeric data types, Tables, Multi-threaded operations, Common program behavior @section Numeric data types @cindex Bit @cindex Type At the lowest level, the computer stores everything in terms of @code{1} or @code{0}. For example, each program in Gnuastro, or each astronomical image you take with the telescope is actually a string of millions of these zeros and ones. The space required to keep a zero or one is the smallest unit of storage, and is known as a @emph{bit}. However, understanding and manipulating this string of bits is extremely hard for most people. Therefore, we define packages of these bits along with a standard on how to interpret the bits in each package as a @emph{type}. @cindex Byte @cindex Signed integer @cindex Unsigned integer @cindex Integer, Signed The most basic standard for reading the bits is integer numbers (@mymath{..., -2, -1, 0, 1, 2, ...}, more bits will give larger limits). The common integer types are 8, 16, 32, and 64 bits wide. For each width, there are two standards for reading the bits: signed and unsigned integers. In the former, negative numbers are allowed and in the latter, they aren't. The @code{unsigned} types thus have larger positive limits (one extra bit), but no negative value. When the context of your work doesn't involve negative numbers (for example counting, where negative is not defined), it is best to use the @code{unsigned} types. For full numerical range of all integer types, see below. Another standard of converting a given number of bits to numbers is the floating point standard, this standard can approximately store any real number with a given precision. There are two common floating point types: 32-bit and 64-bit, for single and double precision floating point numbers respectively. The former is sufficient for data with less than 8 significant decimal digits (most astronomical data), while the latter is good for less than 16 significant decimal digits. The representation of real numbers as bits is much more complex than integers. If you are interested, you can start with the @url{https://en.wikipedia.org/wiki/Floating_point, Wikipedia article}. With the conversion operators in Gnuastro's Arithmetic, you can change the types of data to each other, which is necessary in some contexts. For example the program/library, that you intend to feed the data into, only accepts floating point values, but you have an integer image. Another situation that conversion can be helpful is when you know that your data only has values that fit within @code{int8} or @code{uint16}. However it is currently formatted in the @code{float64} type. Operations involving floating point or larger integer types are significantly slower than integer or smaller-width types respectively. In the latter case, it also requires much more (by 8 or 4 times in the example above) storage space. So when you confront such situations and want to store/archive/transfter the data, it is best convert them to the most efficient type. The short and long names for the recognized numeric data types in Gnuastro are listed below. Both short and long names can be used when you want to specify a type. For example, as a value to the common option @option{--type} (see @ref{Input output options}), or in the information comment lines of @ref{Gnuastro text table format}. The ranges listed below are inclusive. @table @code @item u8 @itemx uint8 8-bit un-signed integers, range:@* @mymath{[0\rm{\ to\ }2^8-1]} or @mymath{[0\rm{\ to\ }255]}. @item i8 @itemx int8 8-bit signed integers, range:@* @mymath{[-2^7\rm{\ to\ }2^7-1]} or @mymath{[-128\rm{\ to\ }127]}. @item u16 @itemx uint16 16-bit un-signed integers, range:@* @mymath{[0\rm{\ to\ }2^{16}-1]} or @mymath{[0\rm{\ to\ }65535]}. @item i16 @itemx int16 16-bit signed integers, range:@* @mymath{[-2^{15}\rm{\ to\ }2^{15}-1]} or @mymath{[-32768\rm{\ to\ }32767]}. @item u32 @itemx uint32 32-bit un-signed integers, range:@* @mymath{[0\rm{\ to\ }2^{32}-1]} or @mymath{[0\rm{\ to\ }4294967295]}. @item i32 @itemx int32 32-bit signed integers, range:@* @mymath{[-2^{31}\rm{\ to\ }2^{31}-1]} or @mymath{[-2147483648\rm{\ to\ }2147483647]}. @item u64 @itemx uint64 64-bit un-signed integers, range@* @mymath{[0\rm{\ to\ }2^{64}-1]} or @mymath{[0\rm{\ to\ }18446744073709551615]}. @item i64 @itemx int64 64-bit signed integers, range:@* @mymath{[-2^{63}\rm{\ to\ }2^{63}-1]} or @mymath{[-9223372036854775808\rm{\ to\ }9223372036854775807]}. @item f32 @itemx float32 32-bit (single-precision) floating point types. The maximum (minimum is its negative) possible value is @mymath{3.402823\times10^{38}}. Single-precision floating points can accurately represent a floating point number up to @mymath{\sim7.2} significant decimals. Given the heavy noise in astronomical data, this is usually more than sufficient for storing results. @item f64 @itemx float64 64-bit (double-precision) floating point types. The maximum (minimum is its negative) possible value is @mymath{\sim10^{308}}. Double-precision floating points can accurately represent a floating point number @mymath{\sim15.9} significant decimals. This is usually good for processing (mixing) the data internally, for example a sum of single precision data (and later storing the result as @code{float32}). @end table @cartouche @noindent @strong{Some file formats don't recognize all types.} Some file formats don't recognize all the types, for example the FITS standard (see @ref{Fits}) does not define @code{uint64} in binary tables or images. When a type is not acceptable for output into a given file format, the respective Gnuastro program or library will let you know and abort. On the command-line, you can use the @ref{Arithmetic} program to convert the numerical type of a dataset, in the libraries, you can call @code{gal_data_copy_to_new_type}. @end cartouche @node Tables, Tessellation, Numeric data types, Common program behavior @section Tables ``A table is a collection of related data held in a structured format within a database. It consists of columns, and rows.'' (from Wikipedia). Each column in the table contains the values of one property and each row is a collection of properties (columns) for one target object. For example, let's assume you have just ran MakeCatalog (see @ref{MakeCatalog}) on an image to measure some properties for the labeled regions (which might be detected galaxies for example) in the image. For each labeled region (detected galaxy), there will be a @emph{row} which groups its measured properties as @emph{columns}, one column for each property. One such property can be the object's magnitude, which is the sum of pixels with that label, or its center can be defined as the light-weighted average value of those pixels. Many such properties can be derived from the raw pixel values and their position, see @ref{Invoking astmkcatalog} for a long list. As a summary, for each labeled region (or, galaxy) we have one @emph{row} and for each measured property we have one @emph{column}. This high-level structure is usually the first step for higher-level analysis, for example finding the stellar mass or photometric redshift from magnitudes in multiple colors. Thus, tables are not just outputs of programs, in fact it is much more common for tables to be inputs of programs. For example, to make a mock galaxy image, you need to feed in the properties of each galaxy into @ref{MakeProfiles} for it do the inverse of the process above and make a simulated image from a catalog, see @ref{Sufi simulates a detection}. In other cases, you can feed a table into @ref{Crop} and it will crop out regions centered on the positions within the table, see @ref{Hubble visually checks and classifies his catalog}. So to end this relatively long introduction, tables play a very important role in astronomy, or generally all branches of data analysis. In @ref{Recognized table formats} the currently recognized table formats in Gnuastro are discussed. You can use any of these tables as input or ask for them to be built as output. The most common type of table format is a simple plain text file with each row on one line and columns separated by white space characters, this format is easy to read/write by eye/hand. To give it the full functionality of more specific table types like the FITS tables, Gnuastro has a special convention which you can use to give each column a name, type, unit, and comments, while still being readable by other plain text table readers. This convention is described in @ref{Gnuastro text table format}. When tables are input to a program, the program reading it needs to know which column(s) it should use for its desired purposes. Gnuastro's programs all follow a similar convention, on the way you can select columns in a table. They are thoroughly discussed in @ref{Selecting table columns}. @menu * Recognized table formats:: Table formats that are recognized in Gnuastro. * Gnuastro text table format:: Gnuastro's convention plain text tables. * Selecting table columns:: Identify/select certain columns from a table @end menu @node Recognized table formats, Gnuastro text table format, Tables, Tables @subsection Recognized table formats The list of table formats that Gnuastro can currently read from and write to are described below. Each has their own advantage and disadvantages, so a short review of the format is also provided to help you make the best choice based on how you want to define your input tables or later use your output tables. @table @asis @item Plain text table This is the most basic and simplest way to create, view, or edit the table by hand on a text editor. The other formats described below are less eye-friendly and have a more formal structure (for easier computer readability). It is fully described in @ref{Gnuastro text table format}. @cindex FITS Tables @cindex Tables FITS @cindex ASCII table, FITS @item FITS ASCII tables The FITS ASCII table extension is fully in ASCII encoding and thus easily readable on any text editor (assuming it is the only extension in the FITS file). If the FITS file also contains binary extensions (for example an image or binary table extensions), then there will be many hard to print characters. The FITS ASCII format doesn't have new line characters to separate rows. In the FITS ASCII table standard, each row is defined as a fixed number of characters (value to the @code{NAXIS1} keyword), so to visually inspect it properly, you would have to adjust your text editor's width to this value. All columns start at given character positions and have a fixed width (number of characters). Numbers in a FITS ASCII table are printed into ASCII format, they are not in binary (that the CPU uses). Hence, they can take a larger space in memory, loose their precision, and take longer to read into memory. If you are dealing with integer type columns (see @ref{Numeric data types}), another issue with FITS ASCII tables is that the type information for the column will be lost (there is only one integer type in FITS ASCII tables). One problem with the binary format on the other hand is that it isn't portable (different CPUs/compilers) have different standards for translating the zeros and ones. But since ASCII characters are defined on a byte and are well recognized, they are better for portability on those various systems. Gnuastro's plain text table format described below is much more portable and easier to read/write/interpret by humans manually. Generally, as the name implies, this format is useful for when your table mainly contains ASCII columns (for example file names, or descriptions). They can be useful when you need to include columns with structured ASCII information along with other extensions in one FITS file. In such cases, you can also consider header keywords (see @ref{Fits}). @cindex Binary table, FITS @item FITS binary tables The FITS binary table is the FITS standard's solution to the issues discussed with keeping numbers in ASCII format as described under the FITS ASCII table title above. Only columns defined as a string type (a string of ASCII characters) are readable in a text editor. The portability problem with binary formats discussed above is mostly solved thanks to the portability of CFITSIO (see @ref{CFITSIO}) and the very long history of the FITS format which has been widely used since the 1970s. In the case of most numbers, storing them in binary format is more memory efficient than ASCII format. For example, to store @code{-25.72034} in ASCII format, you need 9 bytes/characters. But if you keep this same number (to the approximate precision possible) as a 4-byte (32-bit) floating point number, you can keep/transmit it with less than half the amount of memory. When catalogs contain thousands/millions of rows in tens/hundreds of columns, this can lead to significant improvements in memory/band-width usage. Moreover, since the CPU does its operations in the binary formats, reading the table in and writing it out is also much faster than an ASCII table. When you are dealing with integer numbers, the compression ratio can be even better, for example if you know all of the values in a column are positive and less than @code{255}, you can use the @code{unsigned char} type which only takes one byte! If they are between @code{-128} and @code{127}, then you can use the (signed) @code{char} type. So if you are thoughtful about the limits of your integer columns, you can greatly reduce the size of your file and also the speed at which it is read/written. This can be very useful when sharing your results with collaborators or publishing them. To decrease the file size even more you can name your output as ending in @file{.fits.gz} so it is also compressed after creation. Just note that compression/decompressing is CPU intensive and can slow down the writing/reading of the file. Fortunately the FITS Binary table format also accepts ASCII strings as column types (along with the various numerical types). So your dataset can also contain non-numerical columns. @end table @menu * Gnuastro text table format:: Reading plain text tables @end menu @node Gnuastro text table format, Selecting table columns, Recognized table formats, Tables @subsection Gnuastro text table format Plain text files are the most generic, portable, and easiest way to (manually) create, (visually) inspect, or (manually) edit a table. In this format, the ending of a row is defined by the new-line character (a line on a text editor). So when you view it on a text editor, every row will occupy one line. The delimiters (or characters separating the columns) are white space characters (space, horizontal tab, vertical tab) and a comma (@key{,}). The only further requirement is that all rows/lines must have the same number of columns. The columns don't have to be exactly under each other and the rows can be arbitrarily long with different lengths. For example the following contents in a file would be interpreted as a table with 4 columns and 2 rows, with each element interpreted as a @code{double} type (see @ref{Numeric data types}). @example 1 2.234948 128 39.8923e8 2 , 4.454 792 72.98348e7 @end example However, the example above has no other information about the columns (it is just raw data, with no meta-data). To use this table, you have to remember what the numbers in each column represent. Also, when you want to select columns, you have to count their position within the table. This can become frustrating and prone to bad errors (getting the columns wrong) especially as the number of columns increase. It is also bad for sending to a colleague, because they will find it hard to remember/use the columns properly. To solve these problems in Gnuastro's programs/libraries you aren't limited to using the column's number, see @ref{Selecting table columns}. If the columns have names, units, or comments you can also select your columns based on searches/matches in these fields, for example see @ref{Table}. Also, in this manner, you can't guide the program reading the table on how to read the numbers. As an example, the first and third columns above can be read as integer types: the first column might be an ID and the third can be the number of pixels an object occupies in an image. So there is no need to read these to columns as a @code{double} type (which takes more memory, and is slower). In the bare-minimum example above, you also can't use strings of characters, for example the names of filters, or some other identifier that includes non-numerical characters. In the absence of any information, only numbers can be read robustly. Assuming we read columns with non-numerical characters as string, there would still be the problem that the strings might contain space (or any delimiter) character for some rows. So, each `word' in the string will be interpreted as a column and the program will abort with an error that the rows don't have the same number of columns. To correct for these limitations, Gnuastro defines the following convention for storing the table meta-data along with the raw data in one plain text file. The format is primarily designed for ease of reading/writing by eye/fingers, but is also structured enough to be read by a program. When the first non-white character in a line is @key{#}, or there are no non-white characters in it, then the line will not be considered as a row of data in the table (this is a pretty standard convention in many programs, and higher level languages). In the former case, the line is interpreted as a @emph{comment}. If the comment line starts with `@code{# Column N:}', then it is assumed to contain information about column @code{N} (a number, counting from 1). Comment lines that don't start with this pattern are ignored and you can use them to include any further information you want to store with the table in the text file. A column information comment is assumed to have the following format: @example # Column N: NAME [UNIT, TYPE, BLANK] COMMENT @end example @cindex NaN @noindent Any sequence of characters between `@key{:}' and `@key{[}' will be interpreted as the column name (so it can contain anything except the `@key{[}' character). Anything between the `@key{]}' and the end of the line is defined as a comment. Within the brackets, anything before the first `@key{,}' is the units (physical units, for example km/s, or erg/s), anything before the second `@key{,}' is the short type identifier (see below, and @ref{Numeric data types}). Finally (still within the brackets), any non-white characters after the second `@key{,}' are interpreted as the blank value for that column (see @ref{Blank pixels}). Note that blank values will be stored in the same type as the column, not as a string@footnote{For floating point types, the @code{nan}, or @code{inf} strings (both not case-sensitive) refer to IEEE NaN (not a number) and infinity values respectively and will be stored as a floating point, so they are acceptable.}. When a formatting problem occurs (for example you have specified the wrong type code, see below), or the the column was already given meta-data in a previous comment, or the column number is larger than the actual number of columns in the table (the non-commented or empty lines), then the comment information line will be ignored. When a comment information line can be used, the leading and trailing white space characters will be stripped from all of the elements. For example in this line: @example # Column 5: column name [km/s, f32,-99] Redshift as speed @end example The @code{NAME} field will be `@code{column name}' and the @code{TYPE} field will be `@code{f32}'. Note how all the white space characters before and after strings are not used, but those in the middle remained. Also, white space characters aren't mandatory. Hence, in the example above, the @code{BLANK} field will be given the value of `@code{-99}'. Except for the column number (@code{N}), the rest of the fields are optional. Also, the column information comments don't have to be in order. In other words, the information for column @mymath{N+m} (@mymath{m>0}) can be given in a line before column @mymath{N}. Also, you don't have to specify information for all columns. Those columns that don't have this information will be interpreted with the default settings (like the case above: values are double precision floating point, and the column has no name, unit, or comment). So these lines are all acceptable for any table (the first one, with nothing but the column number is redundant): @example # Column 5: # Column 1: ID [,i] The Clump ID. # Column 3: mag_f160w [AB mag, f] Magnitude from the F160W filter @end example @noindent The data type of the column should be specified with one of the following values: @itemize @item For a numeric column, you can use any of the numeric types (and their recognized identifiers) described in @ref{Numeric data types}. @item `@code{strN}': for strings. The @code{N} value identifies the length of the string (how many characters it has). The start of the string on each row is the first non-delimiter character of the column that has the string type. The next @code{N} characters will be interpreted as a string and all leading and trailing white space will be removed. If the next column's characters, are closer than @code{N} characters to the start of the string column in that line/row, they will be considered part of the string column. If there is a new-line character before the ending of the space given to the string column (in other words, the string column is the last column), then reading of the string will stop, even if the @code{N} characters are not complete yet. See @file{tests/table/table.txt} for one example. Therefore, the only time you have to pay attention to the positioning and spaces given to the string column is when it is not the last column in the table. The only limitation in this format is that trailing and leading white space characters will be removed from the columns that are read. In most cases, this is the desired behavior, but if trailing and leading white-spaces are critically important to your analysis, define your own starting and ending characters and remove them after the table has been read. For example in the sample table below, the two `@key{|}' characters (which are arbitrary) will remain in the value of the second column and you can remove them manually later. If only one of the leading or trailing white spaces is important for your work, you can only use one of the `@key{|}'s. @example # Column 1: ID [label, uc] # Column 2: Notes [no unit, str50] 1 leading and trailing white space is ignored here 2.3442e10 2 | but they will be preserved here | 8.2964e11 @end example @end itemize Note that the FITS binary table standard does not define the @code{unsigned int} and @code{unsigned long} types, so if you want to convert your tables to FITS binary tables, use other types. Also, note that in the FITS ASCII table, there is only one integer type (@code{long}). So if you convert a Gnuastro plain text table to a FITS ASCII table with the @ref{Table} program, the type information for integers will be lost. Conversely if integer types are important for you, you have to manually set them when reading a FITS ASCII table (for example with the Table program when reading/converting into a file, or with the @file{gnuastro/table.h} library functions when reading into memory). @node Selecting table columns, , Gnuastro text table format, Tables @subsection Selecting table columns At the lowest level, the only defining aspect of a column in a table is its number, or position. But selecting columns purely by number is not very convenient and, especially when the tables are large it can be very frustrating and prone to errors. Hence, table file formats (for example see @ref{Recognized table formats}) have ways to store additional information about the columns (meta-data). Some of the most common pieces of information about each column are its @emph{name}, the @emph{units} of data in the it, and a @emph{comment} for longer/informal description of the column's data. To facilitate research with Gnuastro, you can select columns by matching, or searching in these three fields, besides the low-level column number. To view the full list of information on the columns in the table, you can use the Table program (see @ref{Table}) with the command below (replace @file{table-file} with the filename of your table, if its FITS, you might also need to specify the HDU/extension which contains the table): @example $ asttable --information table-file @end example Gnuastro's programs need the columns for different purposes, for example in Crop, you specify the columns containing the central coordinates of the crop centers with the @option{--coordcol} option (see @ref{Crop options}). On the other hand, in MakeProfiles, to specify the column containing the profile position angles, you must use the @option{--pcol} option (see @ref{MakeProfiles catalog}). Thus, there can be no unified common option name to select columns for all programs (different columns have different purposes). However, when the program expects a column for a specific context, the option names end in the @option{col} suffix like the examples above. These options accept values in integer (column number), or string (metadata match/search) format. If the value can be parsed as a positive integer, it will be seen as the low-level column number. Note that column counting starts from 1, so if you ask for column 0, the respective program will abort with an error. When the value can't be interpreted as an a integer number, it will be seen as a string of characters which will be used to match/search in the table's meta-data. The meta-data field which the value will be compared with can be selected through the @option{--searchin} option, see @ref{Input output options}. @option{--searchin} can take three values: @code{name}, @code{unit}, @code{comment}. The matching will be done following this convention: @itemize @item If the value is enclosed in two slashes (for example @command{-x/RA_/}, or @option{--coordcol=/RA_/}, see @ref{Crop options}), then it is assumed to be a regular expression with the same convention as GNU AWK. GNU AWK has a very well written @url{https://www.gnu.org/software/gawk/manual/html_node/Regexp.html, chapter} describing regular expressions, so we we will not continue discussing them here. Regular expressions are a very powerful tool in matching text and useful in many contexts. We thus strongly encourage reviewing this chapter for greatly improving the quality of your work in many cases, not just for searching column meta-data in Gnuastro. @item When the string isn't enclosed between `@key{/}'s, any column that exactly matches the given value in the given field will be selected. @end itemize Note that in both cases, you can ignore the case of alphabetic characters with the @option{--ignorecase} option, see @ref{Input output options}. Also, in both cases, multiple columns may be selected with one call to this function. In this case, the order of the selected columns (with one call) will be the same order as they appear in the table. @node Tessellation, Getting help, Tables, Common program behavior @section Tessellation It is sometimes necessary to classify the elements in a dataset (for example pixels in an image) into a grid of individual, non-overlapping tiles. For example when background sky gradients are present in an image, you can define a tile grid over the image. When the tile sizes are set properly, the background's variation over each tile will be negligible, allowing you to measure (and subtract) it. In other cases (for example spatial domain convolution in Gnuastro, see @ref{Convolve}), it might simply be for speed of processing: each tile can be processed independently on a separate CPU thread. In the arts and mathematics, this process is formally known as @url{https://en.wikipedia.org/wiki/Tessellation, tessellation}. The size of the regular tiles (in units of data-elements, or pixels in an image) can be defined with the @option{--tilesize} option. It takes multiple numbers (separated by a comma) which will be the length along the respective dimension (in FORTRAN/FITS dimension order). Divisions are also acceptable, but must result in an integer. For example @option{--tilesize=30,40} can be used for an image (a 2D dataset). The regular tile size along the first FITS axis (horizontal when viewed in SAO ds9) will be 30 pixels and along the second it will be 40 pixels. Ideally, @option{--tilesize} should be selected such that all tiles in the image have exactly the same size. In other words, that the dataset length in each dimension is divisible by the tile size in that dimension. However, this is not always possible: the dataset can be any size and every pixel in it is valuable. In such cases, Gnuastro will look at the significance of the remainder length, if it is not significant (for example one or two pixels), then it will just increase the size of the first tile in the respective dimension and allow the rest of the tiles to have the required size. When the remainder is significant (for example one pixel less than the size along that dimension), the remainder will be added to one regular tile's size and the large tile will be cut in half and put in the two ends of the grid/tessellation. In this way, all the tiles in the central regions of the dataset will have the regular tile sizes and the tiles on the edge will be slightly larger/smaller depending on the remainder significance. The fraction which defines the remainder significance along all dimensions can be set through @option{--remainderfrac}. The best tile size is directly related to the spatial properties of the property you want to study (for example, gradient on the image). In practice we assume that the gradient is not present over each tile. So if there is a strong gradient (for example in long wavelength ground based images) or the image is of a crowded area where there isn't too much blank area, you have to choose a smaller tile size. A larger mesh will give more pixels and and so the scatter in the results will be less (better statistics). @cindex CCD @cindex Amplifier @cindex Bias current @cindex Subaru Telescope @cindex Hyper Suprime-Cam @cindex Hubble Space Telescope For raw image processing, a single tessellation/grid is not sufficient. Raw images are the unprocessed outputs of the camera detectors. Modern detectors usually have multiple readout channels each with its own amplifier. For example the Hubble Space Telescope Advanced Camera for Surveys (ACS) has four amplifiers over its full detector area dividing the square field of view to four smaller squares. Ground based image detectors are not exempt, for example each CCD of Subaru Telescope's Hyper Suprime-Cam camera (which has 104 CCDs) has four amplifiers, but they have the same height of the CCD and divide the width by four parts. @cindex Channel The bias current on each amplifier is different, and initial bias subtraction is not perfect. So even after subtracting the measured bias current, you can usually still identify the boundaries of different amplifiers by eye. See Figure 11(a) in Akhlaghi and Ichikawa (2015) for an example. This results in the final reduced data to have non-uniform amplifier-shaped regions with higher or lower background flux values. Such systematic biases will then propagate to all subsequent measurements we do on the data (for example photometry and subsequent stellar mass and star formation rate measurements in the case of galaxies). Therefore an accurate analysis requires a two layer tessellation: the top layer contains larger tiles, each covering one amplifier channel. For clarity we'll call these larger tiles ``channels''. The number of channels along each dimension is defined through the @option{--numchannels}. Each channel is then covered by its own individual smaller tessellation (with tile sizes determined by the @option{--tilesize} option). This will allow independent analysis of two adjacent pixels from different channels if necessary. If the image is processed or the detector only has one amplifier, you can set the number of channels in both dimension to 1. The final tessellation can be inspected on the image with the @option{--checktiles} option that is available to all programs which use tessellation for localized operations. When this option is called, a FITS file with a @file{_tiled.fits} suffix will be created along with the outputs, see @ref{Automatic output}. Each pixel in this image has the number of the tile that covers it. If the number of channels in any dimension are larger than unity, you will notice that the tile IDs are defined such that the first channels is covered first, then the second and so on. For the full list of processing-related common options (including tessellation options), please see @ref{Processing options}. @node Getting help, Automatic output, Tessellation, Common program behavior @section Getting help @cindex Help @cindex Book formats @cindex Remembering options @cindex Convenient book formats Probably the first time you read this book, it is either in the PDF or HTML formats. These two formats are very convenient for when you are not actually working, but when you are only reading. Later on, when you start to use the programs and you are deep in the middle of your work, some of the details will inevitably be forgotten. Going to find the PDF file (printed or digital) or the HTML webpage is a major distraction. @cindex Online help @cindex Command-line help GNU software have a very unique set of tools for aiding your memory on the command-line, where you are working, depending how much of it you need to remember. In the past, such command-line help was known as ``online'' help, because they were literally provided to you `on' the command `line'. However, nowadays the word ``online'' refers to something on the internet, so that term will not be used. With this type of help, you can resume your exciting research without taking your hands off the keyboard. @cindex Installed help methods Another major advantage of such command-line based help routines is that they are installed with the software in your computer, therefore they are always in sync with the executable you are actually running. Three of them are actually part of the executable. You don't have to worry about the version of the book or program. If you rely on external help (a PDF in your personal print or digital archive or HTML from the official webpage) you have to check to see if their versions fit with your installed program. If you only need to remember the short or long names of the options, @option{--usage} is advised. If it is what the options do, then @option{--help} is a great tool. Man pages are also provided for those who are use to this older system of documentation. This full book is also available to you on the command-line in Info format. If none of these seems to resolve the problems, there is a mailing list which enables you to get in touch with experienced Gnuastro users. In the subsections below each of these methods are reviewed. @menu * --usage:: View option names and value formats. * --help:: List all options with description. * Man pages:: Man pages generated from --help. * Info:: View complete book in terminal. * help-gnuastro mailing list:: Contacting experienced users. @end menu @node --usage, --help, Getting help, Getting help @subsection @option{--usage} @vindex --usage @cindex Usage pattern @cindex Mandatory arguments @cindex Optional and mandatory tokens If you give this option, the program will not run. It will only print a very concise message showing the options and arguments. Everything within square brackets (@option{[]}) is optional. For example here are the first and last two lines of Crop's @option{--usage} is shown: @example $ astcrop --usage Usage: astcrop [-Do?IPqSVW] [-d INT] [-h INT] [-r INT] [-w INT] [-x INT] [-y INT] [-c INT] [-p STR] [-N INT] [--deccol=INT] .... [--setusrconf] [--usage] [--version] [--wcsmode] [ASCIIcatalog] FITSimage(s).fits @end example There are no explanations on the options, just their short and long names shown separately. After the program name, the short format of all the options that don't require a value (on/off options) is displayed. Those that do require a value then follow in separate brackets, each displaying the format of the input they want, see @ref{Options}. Since all options are optional, they are shown in square brackets, but arguments can also be optional. For example in this example, a catalog name is optional and is only required in some modes. This is a standard method of displaying optional arguments for all GNU software. @node --help, Man pages, --usage, Getting help @subsection @option{--help} @vindex --help If the command-line includes this option, the program will not be run. It will print a complete list of all available options along with a short explanation. The options are also grouped by their context. Within each context, the options are sorted alphabetically. Since the options are shown in detail afterwards, the first line of the @option{--help} output shows the arguments and if they are optional or not, similar to @ref{--usage}. In the @option{--help} output of all programs in Gnuastro, the options for each program are classified based on context. The first two contexts are always options to do with the input and output respectively. For example input image extensions or supplementary input files for the inputs. The last class of options is also fixed in all of Gnuastro, it shows operating mode options. Most of these options are already explained in @ref{Operating mode options}. @cindex Long outputs @cindex Redirection of output @cindex Command-line, long outputs The help message will sometimes be longer than the vertical size of your terminal. If you are using a graphical user interface terminal emulator, you can scroll the terminal with your mouse, but we promised no mice distractions! So here are some suggestions: @itemize @item @cindex Scroll command-line @cindex Command-line scroll @cindex @key{Shift + PageUP} and @key{Shift + PageDown} @key{Shift + PageUP} to scroll up and @key{Shift + PageDown} to scroll down. For most help output this should be enough. The problem is that it is limited by the number of lines that your terminal keeps in memory and that you can't scroll by lines, only by whole screens. @item @cindex Pipe @cindex @command{less} Pipe to @command{less}. A pipe is a form of shell re-direction. The @command{less} tool in Unix-like systems was made exactly for such outputs of any length. You can pipe (@command{|}) the output of any program that is longer than the screen to it and then you can scroll through (up and down) with its many tools. For example: @example $ astnoisechisel --help | less @end example @noindent Once you have gone through the text, you can quit @command{less} by pressing the @key{q} key. @item @cindex Save output to file @cindex Redirection of output Redirect to a file. This is a less convenient way, because you will then have to open the file in a text editor! You can do this with the shell redirection tool (@command{>}): @example $ astnoisechisel --help > filename.txt @end example @end itemize @cindex GNU Grep @cindex Searching text @cindex Command-line searching text In case you have a special keyword you are looking for in the help, you don't have to go through the full list. GNU Grep is made for this job. For example if you only want the list of options whose @option{--help} output contains the word ``axis'' in Crop, you can run the following command: @example $ astcrop --help | grep axis @end example @cindex @code{ARGP_HELP_FMT} @cindex Argp argument parser @cindex Customize @option{--help} output @cindex @option{--help} output customization If the output of this option does not fit nicely within the confines of your terminal, GNU does enable you to customize its output through the environment variable @code{ARGP_HELP_FMT}, you can set various parameters which specify the formatting of the help messages. For example if your terminals are wider than 70 spaces (say 100) and you feel there is too much empty space between the long options and the short explanation, you can change these formats by giving values to this environment variable before running the program with the @option{--help} output. You can define this environment variable in this manner: @example $ export ARGP_HELP_FMT=rmargin=100,opt-doc-col=20 @end example @cindex @file{.bashrc} This will affect all GNU programs using GNU C library's @file{argp.h} facilities as long as the environment variable is in memory. You can see the full list of these formatting parameters in the ``Argp User Customization'' part of the GNU C library manual. If you are more comfortable to read the @option{--help} outputs of all GNU software in your customized format, you can add your customizations (similar to the line above, without the @command{$} sign) to your @file{~/.bashrc} file. This is a standard option for all GNU software. @node Man pages, Info, --help, Getting help @subsection Man pages @cindex Man pages Man pages were the Unix method of providing command-line documentation to a program. With GNU Info, see @ref{Info} the usage of this method of documentation is highly discouraged. This is because Info provides a much more easier to navigate and read environment. However, some operating systems require a man page for packages that are installed and some people are still used to this method of command line help. So the programs in Gnuastro also have Man pages which are automatically generated from the outputs of @option{--version} and @option{--help} using the GNU help2man program. So if you run @example $ man programname @end example @noindent You will be provided with a man page listing the options in the standard manner. @node Info, help-gnuastro mailing list, Man pages, Getting help @subsection Info @cindex GNU Info @cindex Command-line, viewing full book Info is the standard documentation format for all GNU software. It is a very useful command-line document viewing format, fully equipped with links between the various pages and menus and search capabilities. As explained before, the best thing about it is that it is available for you the moment you need to refresh your memory on any command-line tool in the middle of your work without having to take your hands off the keyboard. This complete book is available in Info format and can be accessed from anywhere on the command-line. To open the Info format of any installed programs or library on your system which has an Info format book, you can simply run the command below (change @command{executablename} to the executable name of the program or library): @example $ info executablename @end example @noindent @cindex Learning GNU Info @cindex GNU software documentation In case you are not already familiar with it, run @command{$ info info}. It does a fantastic job in explaining all its capabilities its self. It is very short and you will become sufficiently fluent in about half an hour. Since all GNU software documentation is also provided in Info, your whole GNU/Linux life will significantly improve. @cindex GNU Emacs @cindex GNU C library Once you've become an efficient navigator in Info, you can go to any part of this book or any other GNU software or library manual, no matter how long it is, in a matter of seconds. It also blends nicely with GNU Emacs (a text editor) and you can search manuals while you are writing your document or programs without taking your hands off the keyboard, this is most useful for libraries like the GNU C library. To be able to access all the Info manuals installed in your GNU/Linux within Emacs, type @key{Ctrl-H + i}. To see this whole book from the beginning in Info, you can run @example $ info gnuastro @end example @noindent If you run Info with the particular program executable name, for example @file{astcrop} or @file{astnoisechisel}: @example $ info astprogramname @end example @noindent you will be taken to the section titled ``Invoking ProgramName'' which explains the inputs and outputs along with the command-line options for that program. Finally, if you run Info with the official program name, for example Crop or NoiseChisel: @example $ info ProgramName @end example @noindent you will be taken to the top section which introduces the program. Note that in all cases, Info is not case sensitive. @node help-gnuastro mailing list, , Info, Getting help @subsection help-gnuastro mailing list @cindex help-gnuastro mailing list @cindex Mailing list: help-gnuastro Gnuastro maintains the help-gnuastro mailing list for users to ask any questions related to Gnuastro. The experienced Gnuastro users and some of its developers are subscribed to this mailing list and your email will be sent to them immediately. However, when contacting this mailing list please have in mind that they are possibly very busy and might not be able to answer immediately. @cindex Mailing list archives @cindex @code{help-gnuastro@@gnu.org} To ask a question from this mailing list, send a mail to @code{help-gnuastro@@gnu.org}. Anyone can view the mailing list archives at @url{http://lists.gnu.org/archive/html/help-gnuastro/}. It is best that before sending a mail, you search the archives to see if anyone has asked a question similar to yours. If you want to make a suggestion or report a bug, please don't send a mail to this mailing list. We have other mailing lists and tools for those purposes, see @ref{Report a bug} or @ref{Suggest new feature}. @node Automatic output, Output headers, Getting help, Common program behavior @section Automatic output @cindex Automatic output file names @cindex Output file names, automatic @cindex Setting output file names automatically All the programs in Gnuastro are designed such that specifying an output file or directory (based on the program context) is optional. The outputs of most programs are automatically found based on the input and what the program does. For example when you are converting a FITS image named @file{FITSimage.fits} to a JPEG image, the JPEG image will be saved in @file{FITSimage.jpg}. @vindex --keepinputdir Another very important part of the automatic output generation is that all the directory information of the input file name is stripped off of it. This feature can be disabled with the @option{--keepinputdir} option, see @ref{Common options}. It is the default because astronomical data are usually very large and organized specially with special file names. In some cases, the user might not have write permissions in those directories. In fact, even if the data is stored on your own computer, it is advised to only grant write permissions to the super user or root. This way, you won't accidentally delete or modify your valuable data! Let's assume that we are working on a report and want to process the FITS images from two projects (ABC and DEF), which are stored in the sub-directories named @file{ABCproject/} and @file{DEFproject/} of our top data directory (@file{/mnt/data}). The following shell commands show how one image from the former is first converted to a JPEG image through ConvertType and then the objects from an image in the latter project are detected using NoiseChisel. The text after the @command{#} sign are comments (not typed!). @example $ pwd # Current location /home/usrname/research/report $ ls # List directory contents ABC01.jpg $ ls /mnt/data/ABCproject # Archive 1 ABC01.fits ABC02.fits ABC03.fits $ ls /mnt/data/DEFproject # Archive 2 DEF01.fits DEF02.fits DEF03.fits $ astconvertt /mnt/data/ABCproject/ABC02.fits --output=jpg # Prog 1 $ ls ABC01.jpg ABC02.jpg $ astnoisechisel /mnt/data/DEFproject/DEF01.fits # Prog 2 $ ls ABC01.jpg ABC02.jpg DEF01_labeled.fits @end example @node Output headers, , Automatic output, Common program behavior @section Output headers @cindex Output FITS headers @cindex CFITSIO version on outputs The output FITS files created by Gnuastro's programs have some or all of the following standard keywords to keep the basic date and version information of Gnuastro, its dependencies and the pipeline that is using Gnuastro. @table @command @item DATE The creation time of the FITS file. This date is written directly by CFITSIO and is in UT format. @item COMMIT Git's commit description from the running directory of Gnuastro's programs. If the running directory is not version controlled or @file{libgit2} isn't installed (see @ref{Optional dependencies}) then this keyword will not be present. The printed value is equivalent to the output of the following command: @example git describe --dirty --always @end example If the running directory contains non-committed work, then the stored value will have a `@command{-dirty}' suffix. This can be very helpful to let you know that the data is not ready to be shared with collaborators or submitted to a journal. You should only share results that are produced after all your work is committed (safely stored in the version controlled history and thus reproducible). At first sight, version control appears to be mainly a tool for software developers. However progress in a scientific research is almost identical to progress in software development: first you have a rough idea that starts with handful of easy steps. But as the first results appear to be promising, you will have to extend, or generalize, it to make it more robust and work in all the situations your research covers, not just your first test samples. Slowly you will find wrong assumptions or bad implementations that need to be fixed (`bugs' in software development parlance). Finally, when you submit the research to your collaborators or a journal, many comments and suggestions will come in, and you have to address them. Software developers have created version control systems precisely for this kind of activity. Each significant moment in the project's history is called a ``commit'', see @ref{Version controlled source}. A snapshot of the project in each ``commit'' is safely stored away, so you can revert back to it at a later time, or check changes/progress. This way, you can be sure that your work is reproducible and track the progress and history. With version control, experimentation in the project's analysis is greatly facilitated, since you can easily revert back if a brainstorm test procedure fails. One important feature of version control is that the research result (FITS image, table, report or paper) can be stamped with the unique commit information that produced it. This information will enable you to exactly reproduce that same result later, even if you have made changes/progress. For one example of a research paper's reproduction pipeline, please see the @url{https://gitlab.com/makhlaghi/NoiseChisel-paper, reproduction pipeline} of the @url{https://arxiv.org/abs/1505.01664, paper} describing @ref{NoiseChisel}. @item CFITSIO The version of CFITSIO used (see @ref{CFITSIO}). @item WCSLIB The version of WCSLIB used (see @ref{WCSLIB}). Note that older versions of WCSLIB do not report the version internally. So this is only available if you are using more recent WCSLIB versions. @item GSL The version of GNU Scientific Library that was used, see @ref{GNU Scientific Library}. @item GNUASTRO The version of Gnuastro used (see @ref{Version numbering}). @end table Here is one example of the last few lines of an example output. @example / Versions and date DATE = '...' / file creation date COMMIT = 'v0-8-g547f6eb' / Commit description in running dir. CFITSIO = '3.41 ' / CFITSIO version. WCSLIB = '5.16 ' / WCSLIB version. GSL = '2.3 ' / GNU Scientific Library version. GNUASTRO= '0.3' / GNU Astronomy Utilities version. END @end example @node Data containers, Data manipulation, Common program behavior, Top @chapter Data containers @cindex File operations @cindex Operations on files @cindex General file operations The most low-level and basic property of a dataset is how it is stored. To process, archive and transmit the data, you need a container to store it first. From the start of the computer age, different formats have been defined to store data, optimized for particular applications. One format/container can never be useful for all applications: the storage defines the application and vice-versa. In astronomy, the Flexible Image Transport System (FITS) standard has become the most common format of data storage and transmission. It has many useful features, for example multiple sub-containers (also known as extensions or header data units, HDUs) within one file, or support for tables as well as images. Each HDU can store an independent dataset and its corresponding meta-data. Therefore, Gnuastro has one program (see @ref{Fits}) specifically designed to manipulate FITS HDUs and the meta-data (header keywords) in each HDU. Your astronomical research does not just involve data analysis (where the FITS format is very useful). For example you want to demonstrate your raw and processed FITS images or spectra as figures within slides, reports, or papers. The FITS format is not defined for such applications. Thus, Gnuastro also comes with the ConvertType program (see @ref{ConvertType}) which can be used to convert a FITS image to and from (where possible) other formats like plain text and JPEG (which allow two way conversion), along with EPS and PDF (which can only be created from FITS, not the other way round). Finally, the FITS format is not just for images, it can also store tables. Binary tables in particular can be very efficient in storing catalogs that have more than a few tens of columns and rows. However, unlike images (where all elements/pixels have one data type), tables contain multiple columns and each column can have different properties: independent data types (see @ref{Numeric data types}) and meta-data. In practice, each column can be viewed as a separate container that is grouped with others in the table. The only shared property of the columns in a table is thus the number of elements they contain. To allow easy inspection/manipulation of table columns, Gnuastro has the Table program (see @ref{Table}). It can be used to select certain table columns in a FITS table and see them as a human readable output on the command-line, or to save them into another plain text or FITS table. @menu * Fits:: View and manipulate extensions and keywords. * ConvertType:: Convert data to various formats. * Table:: Read and Write FITS tables to plain text. @end menu @node Fits, ConvertType, Data containers, Data containers @section Fits The ``Flexible Image Transport System'', or FITS, is by far the most common data container format in astronomy. Although the full name of the standard invokes the idea that it is only for images, it also contains very complete and robust features for tables. It started off in the 1970s and was formally published as a standard in 1981, it was adopted by the International Astronomical Union (IAU) in 1982 and an IAU working group to maintain its future was defined in 1988. The FITS 2.0 and 3.0 standards were approved in 2000 and 2008 respectively, and the 4.0 draft has also been released recently, please see the @url{https://fits.gsfc.nasa.gov/fits_standard.html, FITS standard document webpage} for the full text of all versions. Also see the @url{https://doi.org/10.1051/0004-6361/201015362, FITS 3.0 standard paper} for a nice introduction and history along with the full standard. @cindex Meta-data Other formats, for example a JPEG image, only have one image/dataset per file, however one great advantage of the FITS standard is that it allows you to keep multiple datasets (images or tables along with their meta-data) in one file. Each data + metadata is known as an extension, or more formally a header data unit or HDU, in the FITS standard. In theory the HDUs can be completely independent: you can have multiple images of different dimensions/sizes or tables as separate extensions in one file. However, while the standard doesn't impose any constraints on the relation between the datasets, it is strongly encouraged to group data that are contextually related with each other in one file. For example an image and the table/catalog of objects and their measured properties in that image. Another example can be multiple images of one patch of sky in different colors (filters). As discussed above, the extensions in a FITS file can be completely independent. To keep some information (meta-data) about the group of extensions in the FITS file, the community has adopted the following convention: put no data in the first extension, so it is just meta-data. This extension can thus be used to store Meta-data regarding the whole file (grouping of extensions). Subsequent extensions may contain data along with their own separate meta-data. All of Gnuastro's programs also follow this convention: the main dataset (image or table) is in the second extension. See the example list of extension properties in @ref{Invoking astfits}. The meta-data contain information about the data, for example which region of the sky an image corresponds to, the units of the data, what telescope, camera, and filter the data were taken with, the software that produced it, or it observation or processing date. Hence without the meta-data, the raw dataset is practically just a collection of numbers and really hard to understand, or connect with the real world (other datasets). It is thus strongly encouraged to supplement your data (at any level of processing) with as much meta-data about your processing/science as possible. The meta-data of a FITS file is in ASCII format, which can be easily viewed or edited with a text editor or on the command-line. Each meta-data element (known as a keyword generally) is composed of a name, value, units and comments (the last two are optional). For example below you can see three FITS meta-data keywords for specifying the world coordinate system (WCS, or its location in the sky) of a dataset: @example LATPOLE = -27.805089 / [deg] Native latitude of celestial pole RADESYS = 'FK5' / Equatorial coordinate system EQUINOX = 2000.0 / [yr] Equinox of equatorial coordinates @end example However, there are some limitations which discourage viewing/editing the keywords with text editors. For example there is a fixed length of 80 characters for each keyword (its name, value, units and comments) and there are no new-line characters, so on a text editor all the keywords are seen in one line. Also, the meta-data keywords are immediately followed by the data which are commonly in binary format and will show up as strange looking characters on a text editor, and significantly slowing down the processor. Gnuastro's Fits program was designed to allow easy manipulation of FITS extensions and meta-data keywords on the command-line while conforming fully with the FITS standard. For example you can copy or cut (copy and remove) HDUs/extensions from one FITS file to another, or completely delete them. It also has features to delete, add, or edit meta-data keywords within one HDU. @menu * Invoking astfits:: Arguments and options to Header. @end menu @node Invoking astfits, , Fits, Fits @subsection Invoking Fits Fits can print or manipulate the FITS file HDUs (extensions), meta-data keywords in a given HDU. The executable name is @file{astfits} with the following general template @example $ astfits [OPTION...] ASTRdata @end example @noindent One line examples: @example ## View general information about every extension: $ astfits image.fits ## Print the header keywords in the second HDU (counting from 0): $ astfits image.fits -h1 ## Only print header keywords that contain `NAXIS': $ astfits image.fits -h1 | grep NAXIS ## Only print the WCS standard PC matrix elements $ astfits image.fits -h1 | grep 'PC._.' ## Copy a HDU from input.fits to out.fits: $ astfits input.fits --copy=hdu-name --output=out.fits ## Update the OLDKEY keyword value to 153.034: $ astfits --update=OLDKEY,153.034,"Old keyword comment" ## Delete one COMMENT keyword and add a new one: $ astfits --delete=COMMENT --comment="Anything you like ;-)." ## Write two new keywords with different values and comments: $ astfits --write=MYKEY1,20.00,"An example keyword" --write=MYKEY2,fd @end example @cindex HDU When no action is requested (and only a file name is given), Fits will print a list of information about the extension(s) in the file. This information includes the HDU number, HDU name (@code{EXTNAME} keyword), type of data (see @ref{Numeric data types}, and the number of data elements it contains (size along each dimension for images and table rows and columns). You can use this to get a general idea of the contents of the FITS file and what HDU to use for further processing, either with the Fits program or any other Gnuastro program. Here is one example of information about a FITS file with four extensions: the first extension has no data, it is a purely meta-data HDU (commonly used to keep meta-data about the whole file, or grouping of extensions, see @ref{Fits}). The second extension is an image with name @code{IMAGE} and single precision floating point type (@code{float32}, see @ref{Numeric data types}), it has 4287 pixels along its first (horizontal) axis and 4286 pixels along its second (vertical) axis. The third extension is also an image with name @code{MASK}. It is in 2-byte integer format (@code{int16}) which is commonly used to keep information about pixels (for example to identify which ones were saturated, or which ones had cosmic rays and so on), note how it has the same size as the @code{IMAGE} extension. The third extension is a binary table called @code{CATALOG} which has 12371 rows and 5 columns (it probably contains information about the sources in the image). @example GNU Astronomy Utilities X.X Run on Day Month DD HH:MM:SS YYYY ----- HDU (extension) information: `image.fits'. Column 1: Index (counting from 0). Column 2: Name (`EXTNAME' in FITS standard). Column 3: Image data type or `table' format (ASCII or binary). Column 4: Size of data in HDU. ----- 0 n/a uint8 0 1 IMAGE float32 4287x4286 2 MASK int16 4287x4286 3 CATALOG table_binary 12371x5 @end example If a specific HDU is identified on the command-line with the @option{--hdu} (or @option{-h} option) and no operation requested, then the full list of header keywords in that HDU will be printed (as if the @option{--printallkeys} was called, see below). It is important to remember that this only occurs when @option{--hdu} is given on the command-line. The @option{--hdu} value given in a configuration file will only be used when a specific operation on keywords requested. Therefore as described in the paragraphs above, when no explicit call to the @option{--hdu} option is made on the command-line and no operation is requested (on the command-line or configuration files), the basic information of each HDU/extension is printed. The operating mode and input/output options to Fits are similar to the other programs and fully described in @ref{Common options}. The options particular to Fits can be divided into two groups: 1) those related to modifying HDUs or extensions (see @ref{HDU manipulation}), and 2) those related to viewing/modifying meta-data keywords (see @ref{Keyword manipulation}). These two classes of options cannot be called together in one run: you can either work on the extensions or meta-data keywords in any instance of Fits. @menu * HDU manipulation:: Manipulate HDUs within a FITS file. * Keyword manipulation:: Manipulate metadata keywords in a HDU @end menu @node HDU manipulation, Keyword manipulation, Invoking astfits, Invoking astfits @subsubsection HDU manipulation Each header data unit, or HDU (also known as an extension), in a FITS file is an independent dataset (data + meta-data). Multiple HDUs can be stored in one FITS file, see @ref{Fits}. The HDU modifying options to the Fits program are listed below. These options may be called multiple times in one run. If so, the extensions will be copied from the input FITS file to the output FITS file in the given order (on the command-line and also in configuration files, see @ref{Configuration file precedence}). If the separate classes are called together in one run of Fits, then first @option{--copy} is run (on all specified HDUs), followed by @option{--cut} (again on all specified HDUs), and then @option{--remove} (on all specified HDUs). The @option{--copy} and @option{--cut} options need an output FITS file (specified with the @option{--output} option). If the output file exists, then the specified HDU will be copied following the last extension of the output file (the existing HDUs in it will be untouched). Thus, after Fits finishes, the copied HDU will be the last HDU of the output file. If no output file name is given, then automatic output will be used to store the HDUs given to this option (see @ref{Automatic output}). @table @option @item -C STR @itemx --copy=STR Copy the specified extension into the output file, see explanations above. @item -k STR @itemx --cut=STR Cut (copy to output, remove from input) the specified extension into the output file, see explanations above. @item -R STR @itemx --remove=STR Remove the specified HDU from the input file. From CFITSIO: ``In the case of deleting the primary array (the first HDU in the file) then [it] will be replaced by a null primary array containing the minimum set of required keywords and no data.''. So in practice, any existing data (array) and meta-data in the first extension will be removed, but the number of extensions in the file won't change. This is because of the unique position the first FITS extension has in the FITS standard (for example it cannot be used to store tables). @end table @node Keyword manipulation, , HDU manipulation, Invoking astfits @subsubsection Keyword manipulation The meta-data in each header data unit, or HDU (also known as extension, see @ref{Fits}) is stored as ``keyword''s. Each keyword consists of a name, value, unit, and comments. The Fits program (see @ref{Fits}) options related to viewing and manipulating keywords in a FITS HDU are described below. To see the full list of keywords in a FITS HDU, you can use the @option{--printallkeys} option. If any of the keywords are to be modified, the headers of the input file will be changed. If you want to keep the original FITS file or HDU, it is easiest to create a copy first and then run Fits on that. In the FITS standard, keywords are always uppercase. So case does not matter in the input or output keyword names you specify. Most of the options can accept multiple instances in one command. For example you can add multiple keywords to delete by calling @option{--delete} multiple times, since repeated keywords are allowed, you can even delete the same keyword multiple times. The action of such options will start from the top most keyword. The precedence of operations are described below. Note that while the order within each class of actions is preserved, the order of individual actions is not. So irrespective of what order you called @option{--delete} and @option{--update}. First, all the delete operations are going to take effect then the update operations. @enumerate @item @option{--delete} @item @option{--rename} @item @option{--update} @item @option{--write} @item @option{--asis} @item @option{--history} @item @option{--comment} @item @option{--date} @item @option{--printallkeys} @end enumerate @noindent All possible syntax errors will be reported before the keywords are actually written. FITS errors during any of these actions will be reported, but Fits won't stop until all the operations are complete. If @option{--quitonerror} is called, then Fits will immediately stop upon the first error. @cindex GNU Grep If you want to inspect only a certain set of header keywords, it is easiest to pipe the output of the Fits program to GNU Grep. Grep is a very powerful and advanced tool to search strings which is precisely made for such situations. For example if you only want to check the size of an image FITS HDU, you can run: @example $ astfits input.fits | grep NAXIS @end example @cartouche @noindent @strong{FITS STANDARD KEYWORDS:} Some header keywords are necessary for later operations on a FITS file, for example BITPIX or NAXIS, see the FITS standard for their full list. If you modify (for example remove or rename) such keywords, the FITS file extension might not be usable any more. Also be careful for the world coordinate system keywords, if you modify or change their values, any future world coordinate system (like RA and Dec) measurements on the image will also change. @end cartouche @noindent The keyword related options to the Fits program are fully described below. @table @option @item -a STR @itemx --asis=STR Write @option{STR} exactly into the FITS file header with no modifications. If it does not conform to the FITS standards, then it might cause trouble, so please be very careful with this option. If you want to define the keyword from scratch, it is best to use the @option{--write} option (see below) and let CFITSIO worry about the standards. The best way to use this option is when you want to add a keyword from one FITS file to another unchanged and untouched. Below is an example of such a case that can be very useful sometimes (on the command-line or in scripts): @example $ key=$(astfits firstimage.fits | grep KEYWORD) $ astfits --asis="$key" secondimage.fits @end example @cindex GNU Bash In particular note the double quotation signs (@key{"}) around the reference to the @command{key} shell variable (@command{$key}), since FITS keywords usually have lots of space characters, if this variable is not quoted, the shell will only give the first word in the full keyword to this option, which will definitely be a non-standard FITS keyword and will make it hard to work on the file afterwords. See the ``Quoting'' section of the GNU Bash manual for more information if your keyword has the special characters @key{$}, @key{`}, or @key{\}. @item -d STR @itemx --delete=STR Delete one instance of the @option{STR} keyword from the FITS header. Multiple instances of @option{--delete} can be given (possibly even for the same keyword, when its repeated in the meta-data). All keywords given will be removed from the headers in the same given order. If the keyword doesn't exist, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with @option{--quitonerror}. @item -r STR @itemx --rename=STR Rename a keyword to a new value. @option{STR} contains both the existing and new names, which should be separated by either a comma (@key{,}) or a space character. Note that if you use a space character, you have to put the value to this option within double quotation marks (@key{"}) so the space character is not interpreted as an option separator. Multiple instances of @option{--rename} can be given in one command. The keywords will be renamed in the specified order. If the keyword doesn't exist, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with @option{--quitonerror}. @item -u STR @itemx --update=STR Update a keyword, its value, its comments and its units in the format described below. If there are multiple instances of the keyword in the header, they will be changed from top to bottom (with multiple @option{--update} options). @noindent The format of the values to this option can best be specified with an example: @example --update=KEYWORD,value,"comments for this keyword",unit @end example If there is a writing error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with @option{--quitonerror}. @noindent The value can be any numerical or string value@footnote{Some tricky situations arise with values like `@command{87095e5}', if this was intended to be a number it will be kept in the header as @code{8709500000} and there is no problem. But this can also be a shortened Git commit hash. In the latter case, it should be treated as a string and stored as it is written. Commit hashes are very important in keeping the history of a file during your research and such values might arise without you noticing them in your reproduction pipeline. One solution is to use @command{git describe} instead of the short hash alone. A less recommended solution is to add a space after the commit hash and Fits will write the value as `@command{87095e5 }' in the header. If you later compare the strings on the shell, the space character will be ignored by the shell in the latter solution and there will be no problem.}. Other than the @code{KEYWORD}, all the other values are optional. To leave a given token empty, follow the preceding comma (@key{,}) immediately with the next. If any space character is present around the commas, it will be considered part of the respective token. So if more than one token has space characters within it, the safest method to specify a value to this option is to put double quotation marks around each individual token that needs it. Note that without double quotation marks, space characters will be seen as option separators and can lead to undefined behavior. @item -w STR @itemx --write=STR Write a keyword to the header. For the possible value input formats, comments and units for the keyword, see the @option{--update} option above. @item -H STR @itemx --history STR Add a @code{HISTORY} keyword to the header. The string given to this keyword will be separated into multiple keyword cards if it is longer than 70 characters. With each run only one value for the @option{--history} option will be read. If there are multiple, it is the last one. If there is an error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with @option{--quitonerror}. @item -c STR @itemx --comment STR Add a @code{COMMENT} keyword to the header. Similar to the explanation for @option{--history} above. If there is a writing error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with @option{--quitonerror}. @item -t @itemx --date Put the current date and time in the header. If the @code{DATE} keyword already exists in the header, it will be updated. If there is a writing error, Fits will give a warning and return with a non-zero value, but will not stop. To stop as soon as an error occurs, run with @option{--quitonerror}. @item -p @itemx --printall Print all the keywords in the specified FITS extension (HDU) on the command-line. @item -Q @itemx --quitonerror Quit if any of the operations above are not successful. By default if an error occurs, Fits will warn the user of the faulty keyword and continue with the rest of actions. @end table @node ConvertType, Table, Fits, Data containers @section ConvertType @cindex Data format conversion @cindex Converting data formats @cindex Image format conversion @cindex Converting image formats @pindex @r{ConvertType (}astconvertt@r{)} The formats of astronomical data were defined mainly for archiving and processing. In other situations, the data might be useful in other formats. For example, when you are writing a paper or report or if you are making slides for a talk, you can't use a FITS image. Other image formats should be used. In other cases you might want your pixel values in a table format as plain text for input to other programs that don't recognize FITS, or to include as a table in your report. ConvertType is created for such situations. The various types will increase with future updates and based on need. The conversion is not only one way (from FITS to other formats), but two ways (except the EPS and PDF formats). So you can convert a JPEG image or text file into a FITS image. Basically, other than EPS, you can use any of the recognized formats as different color channel inputs to get any of the recognized outputs. So before explaining the options and arguments, first a short description of the recognized files types will be given followed a short introduction to digital color. @menu * Recognized file formats:: Recognized file formats * Color:: Some explanations on color. * Invoking astconvertt:: Options and arguments to ConvertType. @end menu @node Recognized file formats, Color, ConvertType, ConvertType @subsection Recognized file formats The various standards and the file name extensions recognized by ConvertType are listed below. @table @asis @item FITS or IMH @cindex Astronomical data format Astronomical data are commonly stored in the FITS format (and in older data sets in IRAF @file{.imh} format), a list of file name suffixes which indicate that the file is in this format is given in @ref{Arguments}. Each extension of a FITS image only has one value per pixel, so when used as input, each input FITS image contributes as one color channel. If you want multiple extensions in one FITS file for different color channels, you have to repeat the file name multiple times and use the @option{--hdu}, @option{--hdu2}, @option{--hdu3} or @option{--hdu4} options to specify the different extensions. @item JPEG @cindex JPEG format @cindex Raster graphics @cindex Pixelated graphics The JPEG standard was created by the Joint photographic experts group. It is currently one of the most commonly used image formats. Its major advantage is the compression algorithm that is defined by the standard. Like the FITS standard, this is a raster graphics format, which means that it is pixelated. A JPEG file can have 1 (for gray-scale), 3 (for RGB) and 4 (for CMYK) color channels. If you only want to convert one JPEG image into other formats, there is no problem, however, if you want to use it in combination with other input files, make sure that the final number of color channels does not exceed four. If it does, then ConvertType will abort and notify you. @cindex Suffixes, JPEG images The file name endings that are recognized as a JPEG file for input are: @file{.jpg}, @file{.JPG}, @file{.jpeg}, @file{.JPEG}, @file{.jpe}, @file{.jif}, @file{.jfif} and @file{.jfi}. @item EPS @cindex EPS @cindex PostScript @cindex Vector graphics @cindex Encapsulated PostScript The Encapsulated PostScript (EPS) format is essentially a one page PostScript file which has a specified size. PostScript also includes non-image data, for example lines and texts. It is a fully functional programming language to describe a document. Therefore in ConvertType, EPS is only an output format and cannot be used as input. Contrary to the FITS or JPEG formats, PostScript is not a raster format, but is categorized as vector graphics. @cindex PDF @cindex Adobe systems @cindex PostScript vs. PDF @cindex Compiled PostScript @cindex Portable Document format @cindex Static document description format The Portable Document Format (PDF) is currently the most common format for documents. Some believe that PDF has replaced PostScript and that PostScript is now obsolete. This view is wrong, a PostScript file is an actual plain text file that can be edited like any program source with any text editor. To be able to display its programmed content or print, it needs to pass through a processor or compiler. A PDF file can be thought of as the processed output of the compiler on an input PostScript file. PostScript, EPS and PDF were created and are registered by Adobe Systems. @cindex @TeX{} @cindex @LaTeX{} With these features in mind, you can see that when you are compiling a document with @TeX{} or @LaTeX{}, using an EPS file is much more low level than a JPEG and thus you have much greater control and therefore quality. Since it also includes vector graphic lines we also use such lines to make a thin border around the image to make its appearance in the document much better. No matter the resolution of the display or printer, these lines will always be clear and not pixelated. In the future, addition of text might be included (for example labels or object IDs) on the EPS output. However, this can be done better with tools within @TeX{} or @LaTeX{} such as PGF/Tikz@footnote{@url{http://sourceforge.net/projects/pgf/}}. @cindex Binary image @cindex Saving binary image @cindex Black and white image If the final input image (possibly after all operations on the flux explained below) is a binary image or only has two colors of black and white (in segmentation maps for example), then PostScript has another great advantage compared to other formats. It allows for 1 bit pixels (pixels with a value of 0 or 1), this can decrease the output file size by 8 times. So if a gray-scale image is binary, ConvertType will exploit this property in the EPS and PDF (see below) outputs. @cindex Suffixes, EPS format The standard formats for an EPS file are @file{.eps}, @file{.EPS}, @file{.epsf} and @file{.epsi}. The EPS outputs of ConvertType have the @file{.eps} suffix. @item PDF @cindex Suffixes, PDF format @cindex GPL Ghostscript As explained above, a PDF document is a static document description format, viewing its result is therefore much faster and more efficient than PostScript. To create a PDF output, ConvertType will make a PostScript page description and convert that to PDF using GPL Ghostscript. The suffixes recognized for a PDF file are: @file{.pdf}, @file{.PDF}. If GPL Ghostscript cannot be run on the PostScript file, it will remain and a warning will be printed. @item @option{blank} @cindex @file{blank} color channel This is not actually a file type! But can be used to fill one color channel with a blank value. If this argument is given for any color channel, that channel will not be used in the output. @item Plain text @cindex Plain text @cindex Suffixes, plain text Plain text files have the advantage that they can be viewed with any text editor or on the command-line. Most programs also support input as plain text files. As input, each plain text file is considered to contain one color channel. In ConvertType, the recognized extensions for plain text files are @file{.txt} and @file{.dat}. As described in @ref{Invoking astconvertt}, if you just give these extensions, (and not a full filename) as output, then automatic output will be preformed to determine the final output name (see @ref{Automatic output}). Besides these, when the format of a file cannot be recognized from its name, ConvertType will fall back to plain text mode. So you can use any name (even without an extension) for a plain text input or output. Just note that when the suffix is not recognized, automatic output will not be preformed. The basic input/output on plain text images is very similar to how tables are read/written as described in @ref{Gnuastro text table format}. Simply put, the restrictions are very loose, and there is a convention to define a name, units, data type (see @ref{Numeric data types}), and comments for the data in a commented line. The only difference is that as a table, a text file can contain many datasets (columns), but as a 2D image, it can only contain one dataset. As a result, only one information comment line is necessary for a 2D image, and instead of the starting `@code{# Column N}' (@code{N} is the column number), the information line for a 2D image must start with `@code{# Image 1}'. When ConvertType is asked to output to plain text file, this information comment line is written before the image pixel values. When converting an image to plain text, consider the fact that if the image is large, the number of columns in each line will become very large, possibly making it very hard to open in some text editors. @item Standard output (command-line) This is very similar to the plain text output, but instead of creating a file to keep the printed values, they are printed on the command line. This can be very useful when you want to redirect the results directly to another program in one command with no intermediate file. The only difference is that only the pixel values are printed (with no information comment line). To print to the standard output, set the output name to `@file{stdout}'. @end table @node Color, Invoking astconvertt, Recognized file formats, ConvertType @subsection Color @cindex RGB @cindex CMYK @cindex Image @cindex Pixels @cindex Grayscale @cindex Colorspace @cindex Primary colors @cindex Colorspace, gray-scale An image is a two dimensional array of 2 dimensional elements called pixels. If each pixel only has one value, the image is known as a gray-scale image and no color is defined. The range of values in the image can be interpreted as shades of any color, it is customary to use shades of black or gray-scale. However, to produce the color spectrum in the digital world, several primary colors must be mixed. Therefore in a color image, each pixel has several values depending on how many primary colors were chosen. For example on the digital monitor or color digital cameras, all colors are built by mixing the three colors of Red-Green-Blue (RGB) with various proportions. However, for printing on paper, standard printers use the Cyan-Magenta-Yellow-Key (CMYK, Key=black) color space. Therefore when printing an RGB image, usually a transformation of color spaces will be necessary. In a colored digital camera, a color image is produced by dividing the pixel's area between three colors (filters). However in astronomy due to the intrinsic faintness of most of the targets, the collecting area of the pixel is very important for us. Hence the full area of the pixel is used and one value is stored for that pixel in the end. One color filter is used for the whole image. Thus a FITS image is inherently a gray-scale image and no color can be defined for it. @cindex Colorspace, transformation One way to represent a gray-scale image in different color spaces is to use the same proportions of the primary colors in each pixel. This is the common way most FITS image converters work: they fill all the channels with the same values. The downside is two fold: @itemize @item Three (for RGB) or four (for CMYK) values have to be stored for every pixel, this makes the output file very heavy (in terms of bytes). @item If printing, the printing errors of each color channel can make the printed image slightly more blurred than it actually is. @end itemize @cindex PNG standard @cindex Single channel CMYK To solve both these problems, the best way is to save the FITS image into the black channel of the CMYK color space. In the RGB color space all three channels have to be used. The JPEG standard is the only common standard that accepts CMYK color space, that is why currently only the JPEG standard is included and not the PNG standard for example. The JPEG and EPS standards set two sizes for the number of bits in each channel: 8-bit and 12-bit. The former is by far the most common and is what is used in ConvertType. Therefore, each channel should have values between 0 to @math{2^8-1=255}. From this we see how each pixel in a gray-scale image is one byte (8 bits) long, in an RGB image, it is 3bytes long and in CMYK it is 4bytes long. But thanks to the JPEG compression algorithms, when all the pixels of one channel have the same value, that channel is compressed to one pixel. Therefore a Grayscale image and a CMYK image that has only the K-channel filled are approximately the same file size. @node Invoking astconvertt, , Color, ConvertType @subsection Invoking ConvertType ConvertType will convert any recognized input file type to any specified output type. The executable name is @file{astconvertt} with the following general template @example $ astconvertt [OPTION...] InputFile [InputFile2] ... [InputFile4] @end example @noindent One line examples: @example ## Convert an image in FITS to PDF: $ astconvertt image.fits --output=pdf ## Convert an image in JPEG to FITS: $ astconvertt image.jpg -ogalaxy.fits ## Use three plain text 2D arrays to create an RGB JPEG output: $ astconvertt f1.txt f2.txt f3.fits -o.jpg ## Use two images and one blank for an RGB EPS output: $ astconvertt M31_r.fits M31_g.fits blank -oeps @end example @noindent The file type of the output will be specified with the (possibly complete) file name given to the @option{--output} option, which can either be given on the command-line or in any of the configuration files (see @ref{Configuration files}). Note that if the output suffix is not recognized, it will default to plain text format, see @ref{Recognized file formats}. The order of multiple input files is important. After reading the input file(s) the number of color channels in all the inputs will be used to define which color space is being used for the outputs and how each color channel is interpreted. Note that one file might have more than one color channel (for example in the JPEG format). If there is one color channel the output is gray-scale, if three input color channels are given they are respectively considered to be the red, green and blue color channels and if there are four color channels they are respectively considered to be cyan, magenta, yellow and black. The value to @option{--output} (or @option{-o}) can be either a full file name or just the suffix of the desired output format. In the former case, that same name will be used for the output. In the latter case, the name of the output file will be set based on the automatic output guidelines, see @ref{Automatic output}. Note that the suffix name can optionally start a @file{.} (dot), so for example @option{--output=.jpg} and @option{--output=jpg} are equivalent. See @ref{Recognized file formats} Besides the common set of options explained in @ref{Common options}, the options to ConvertType can be classified into input, output and flux related options. The majority of the options are to do with the flux range. Astronomical data usually have a very large dynamic range (difference between maximum and minimum value) and different subjects might be better demonstrated with a limited flux range. @noindent Input: @table @option @item -h STR/INT @itemx --hdu=STR/INT In ConvertType, it is possible to call the HDU option multiple times for the different input FITS files (corresponding to different color channels) in the same order that they are called on the command-line. Except for the fact that multiple calls are possible, this option is identical to the common @option{--hdu} in @ref{Input output options}. The number of calls to this option cannot be less than the number of input FITS files, but if there are more, the extra HDUs will be ignored, note that they will be read in the order described in @ref{Configuration file precedence}. @end table @noindent Output: @table @option @item -w FLT @itemx --widthincm=FLT The width of the output in centimeters. This is only relevant for those formats that accept such a width (not plain text for example). For most digital purposes, the number of pixels is far more important than the value to this parameter because you can adjust the absolute width (in inches or centimeters) in your document preparation program. @item -b INT @itemx --borderwidth=INT @cindex Border on an image The width of the border to be put around the EPS and PDF outputs in units of PostScript points. There are 72 or 28.35 PostScript points in an inch or centimeter respectively. In other words, there are roughly 3 PostScript points in every millimeter. If you are planning on adding a border, its significance is highly correlated with the value you give to the @option{--widthincm} parameter. Unfortunately in the document structuring convention of the PostScript language, the ``bounding box'' has to be in units of PostScript points with no fractions allowed. So the border values only have to be specified in integers. To have a final border that is thinner than one PostScript point in your document, you can ask for a larger width in ConvertType and then scale down the output EPS or PDF file in your document preparation program. For example by setting @command{width} in your @command{includegraphics} command in @TeX{} or @LaTeX{}. Since it is vector graphics, the changes of size have no effect on the quality of your output quality (pixels don't get different values). @item -x @itemx --hex @cindex ASCII85 encoding @cindex Hexadecimal encoding Use Hexadecimal encoding in creating EPS output. By default the ASCII85 encoding is used which provides a much better compression ratio. When converted to PDF (or included in @TeX{} or @LaTeX{} which is finally saved as a PDF file), an efficient binary encoding is used which is far more efficient than both of them. The choice of EPS encoding will thus have no effect on the final PDF. So if you want to transfer your EPS files (for example if you want to submit your paper to arXiv or journals in PostScript), their storage might become important if you have large images or lots of small ones. By default ASCII85 encoding is used which offers a much better compression ratio (nearly 40 percent) compared to Hexadecimal encoding. @item -u INT @itemx --quality=INT @cindex JPEG compression quality @cindex Compression quality in JPEG @cindex Quality of compression in JPEG The quality (compression) of the output JPEG file with values from 0 to 100 (inclusive). For other formats the value to this option is ignored. Note that only in gray-scale (when one input color channel is given) will this actually be the exact quality (each pixel will correspond to one input value). If it is in color mode, some degradation will occur. While the JPEG standard does support loss-less graphics, it is not commonly supported. @end table @noindent Flux range: @table @option @item -c STR @itemx --chang=STR @cindex Change converted pixel values (@option{=STR}) Change pixel values with the following format @option{"from1:to1, from2:to2,..."}. This option is very useful in displaying labeled pixels (not actual data images which have noise) like segmentation maps. In labeled images, usually a group of pixels have a fixed integer value. With this option, you can manipulate the labels before the image is displayed to get a better output for print or to emphasize on a particular set of labels and ignore the rest. The labels in the images will be changed in the same order given. By default first the pixel values will be converted then the pixel values will be truncated (see @option{--fluxlow} and @option{--fluxhigh}). You can use any number for the values irrespective of your final output, your given values are stored and used in the double precision floating point format. So for example if your input image has labels from 1 to 20000 and you only want to display those with labels 957 and 11342 then you can run ConvertType with these options: @example $ astconvertt --change=957:50000,11342:50001 --fluxlow=5e4 \ --fluxhigh=1e5 segmentationmap.fits --output=jpg @end example @noindent While the output JPEG format is only 8 bit, this operation is done in an intermediate step which is stored in double precision floating point. The pixel values are converted to 8-bit after all operations on the input fluxes have been complete. By placing the value in double quotes you can use as many spaces as you like for better readability. @item -C @itemx --changeaftertrunc Change pixel values (with @option{--change}) after truncation of the flux values, by default it is the opposite. @item -L FLT @itemx --fluxlow=FLT The minimum flux (pixel value) to display in the output image, any pixel value below this value will be set to this value in the output. If the value to this option is the same as @option{--fluxmax}, then no flux truncation will be applied. Note that when multiple channels are given, this value is used for all the color channels. @item -H FLT @itemx --fluxhigh=FLT The maximum flux (pixel value) to display in the output image, see @option{--fluxlow}. @item -m INT @itemx --maxbyte=INT This is only used for the JPEG and EPS output formats which have an 8-bit space for each channel of each pixel. The maximum value in each pixel can therefore be @mymath{2^8-1=255}. With this option you can change (decrease) the maximum value. By doing so you will decrease the dynamic range. It can be useful if you plan to use those values for other purposes. @item -A INT @itemx --flminbyte=INT If the lowest pixel value in the input channels is larger than the value to @option{--fluxlow}, then that input value will be redundant. In some situations it might be necessary to set the minimum byte value (0) to correspond to that flux even if the data do not reach that value. With this option you can do this. Note that if the minimum pixel value is smaller than @option{--fluxlow}, then this option is redundant. @item -B INT @itemx --fhmaxbyte=INT See @option{--flminbyte}. @item -i @itemx --invert For 8-bit output types (JPEG, EPS, and PDF for example) the final value that is stored is inverted so white becomes black and vice versa. The reason for this is that astronomical images usually have a very large area of blank sky in them. The result will be that a large are of the image will be black. Note that this behavior is ideal for gray-scale images, if you want a color image, the colors are going to be mixed up. @end table @node Table, , ConvertType, Data containers @section Table Tables are the products of processing astronomical images and spectra. For example in Gnuastro, MakeCatalog will process the defined pixels over an object and produce a catalog (see @ref{MakeCatalog}). For each identified object, MakeCatalog can print its position on the image or sky, its total brightness and many other information that is deducible from the given image. Each one of these properties is a column in its output catalog (or table) and for each input object, we have a row. When there are only a small number of objects (rows) and not too many properties (columns), then a simple plain text file is mainly enough to store, transfer, or even use the produced data. However, to be more efficient in all these aspects, astronomers have defined the FITS binary table standard to store data in a binary (0 and 1) format, not plain text. This can offer major advantages in all those aspects: the file size will be greatly reduced and the reading and writing will be faster (because the RAM and CPU also work in binary). The FITS standard also defines a standard for ASCII tables, where the data are stored in the human readable ASCII format, but within the FITS file structure. These are mainly useful for keeping ASCII data along with images and possibly binary data as multiple (conceptually related) extensions within a FITS file. The acceptable table formats are fully described in @ref{Tables}. @cindex AWK @cindex GNU AWK Binary tables are not easily readable by human eyes. There is no fixed/unified standard on how the zero and ones should be interpreted. The Unix-like operating systems have flourished because of a simple fact: communication between the various tools is based on human readable characters@footnote{In ``The art of Unix programming'', Eric Raymond makes this suggestion to programmers: ``When you feel the urge to design a complex binary file format, or a complex binary application protocol, it is generally wise to lie down until the feeling passes.''. This is a great book and strongly recommended, give it a look if you want to truly enjoy your work/life in this environment.}. So while the FITS table standards are very beneficial for the tools that recognize them, they are hard to use in the vast majority of available software. This creates limitations for their generic use. `Table' is Gnuastro's solution to this problem. With Table, FITS tables (ASCII or binary) are directly accessible to the Unix-like operating systems power-users (those working the command-line or shell, see @ref{Command-line interface}). With Table, a FITS table (in binary or ASCII formats) is only one command away from AWK (or any other tool you want to use). Just like a plain text file that you read with the @command{cat} command. You can pipe the output of Table into any other tool for higher-level processing, see the examples in @ref{Invoking asttable} for some simple examples. @menu * Invoking asttable:: Options and arguments to Table. @end menu @node Invoking asttable, , Table, Table @subsection Invoking Table Table will read/write, select, convert, or show the information of the columns in FITS ASCII table, FITS binary table and plain text table files, see @ref{Tables}. Output columns can also be determined by number or regular expression matching of column names, units, or comments. The executable name is @file{asttable} with the following general template @example $ asttable [OPTION...] InputFile @end example @noindent One line examples: @example ## Get the table column information (name, data type, or units): $ asttable bintab.fits --information ## Only print those columns which have a name starting with "MAG_": $ asttable bintab.fits --column=/^MAG_/ ## Only print the 2nd column, and the third column multiplied by 5: $ asttable bintab.fits | awk '@{print $2, 5*$3@}' ## Only print rows with a value in the 10th column above 100000: $ asttable bintab.fits | awk '$10>10e5 @{print@}' ## Sort the output columns by the third column, save output: $ asttable bintab.fits | 'sort -k3 > output.txt ## Convert a plain text table to a binary FITS table: $ asttable plaintext.txt --output=table.fits --tabletype=fits-binary @end example @cindex GNU AWK In the absence of selected columns, all the input file's columns will be output. If the specified output is a FITS file, the type of FITS table (binary or ASCII) will be determined from the @option{--tabletype} option. If the output is not a FITS file, it will be printed as a plain text table (with space characters between the columns). When the columns are accompanied by meta-data (like column name, units, or comments), this information will also printed in the plain text file before the table, as described in @ref{Gnuastro text table format}. For the full list of options common to all Gnuastro programs please see @ref{Common options}. Options can also be stored in directory, user or system-wide configuration files to avoid repeating on the command-line, see @ref{Configuration files}. Table does not follow Automatic output that is common in most Gnuastro programs, see @ref{Automatic output}. Thus, in the absence of an output file, the selected columns will be printed on the command-line with no column information, ready for redirecting to other tools like AWK or sort, similar to the examples above. @table @option @item -i @itemx --information Only print the column information in the specified table on the command-line and exit. Each column's information (number, name, units, data type, and comments) will be printed as a row on the command-line. Note that the FITS standard only requires the data type (see @ref{Numeric data types}), and in plain text tables, no meta-data/information is mandatory. Gnuastro has its own convention in the comments of a plain text table to store and transfer this information as described in @ref{Gnuastro text table format}. This option will take precedence over the @option{--column} option, so when it is called along with requested columns, the latter will be ignored. This can be useful if you forget the identifier of a column after you have already typed some on the command-line. You can simply add a @option{-i} and run Table to see the whole list and remember. Then you can use the shell history (with the up arrow key on the keyboard), and retrieve the last command with all the previously typed columns present, delete @option{-i} and add the identifier you had forgot. @cindex AWK @cindex GNU AWK @item -c STR/INT @itemx --column=STR/INT Specify the columns to output, see @ref{Selecting table columns} for a thorough explanation on how the value to this option is interpreted. To select several output columns, this option can also be called any number times in one call to Table. The order of the output columns will be the same call order on the command-line. This option is not mandatory, if no specific columns are requested, all the input table columns are output. When this option is called multiple times, it is possible to output one column more than once. @end table @node Data manipulation, Data analysis, Data containers, Top @chapter Data manipulation Images are one of the major formats of data that is used in astronomy. The functions in this chapter explain the GNU Astronomy Utilities which are provided for their manipulation. For example cropping out a part of a larger image or convolving the image with a given kernel or applying a transformation to it. @menu * Crop:: Crop region(s) from a dataset. * Arithmetic:: Arithmetic on input data. * Convolve:: Convolve an image with a kernel. * Warp:: Warp/Transform an image to a different grid. @end menu @node Crop, Arithmetic, Data manipulation, Data manipulation @section Crop @cindex Section of an image @cindex Crop part of image @cindex Postage stamp images @cindex Large astronomical images @pindex @r{Crop (}astcrop@r{)} Astronomical images are often very large, filled with thousands of galaxies. It often happens that you only want a section of the image, or you have a catalog of sources and you want to visually analyze them in small postage stamps. Crop is made to do all these things. When more than one crop is required, Crop will divide the crops between multiple threads to significantly reduce the run time. @cindex Mosaicing @cindex Image tiles @cindex Image mosaic @cindex COSMOS survey @cindex Imaging surveys @cindex Hubble Space Telescope Astronomical surveys are usually extremely large. So large in fact, that the whole survey will not fit into a reasonably sized file. Because of this, surveys usually cut the final image into separate tiles and store each tile in a file. For example the COSMOS survey's Hubble space telescope, ACS F814W image consists of 81 separate FITS images, with each one having a volume of 1.7 Giga bytes. @cindex Stitch multiple images Even though the tile sizes are chosen to be large enough that too many galaxies/targets don't fall on the edges of the tiles, inevitably some do. So when you simply crop the image of such targets from one tile, you will miss a large area of the surrounding sky (which is essential in estimating the noise). Therefore in its WCS mode, Crop will stitch parts of the tiles that are relevant for a target (with the given width) from all the input images that cover that region into the output. Of course, the tiles have to be present in the list of input files. Besides cropping postage stamps around certain coordinates, Crop can also crop arbitrary polygons from an image (or a set of tiles by stitching the relevant parts of different tiles within the polygon), see @option{--polygon} in @ref{Invoking astcrop}. Alternatively, it can crop out rectangular regions through the @option{--section} option from one image, see @ref{Crop section syntax}. @menu * Crop modes:: Basic modes to define crop region. * Crop section syntax:: How to define a section to crop. * Blank pixels:: Pixels with no value. * Invoking astcrop:: Calling Crop on the command-line @end menu @node Crop modes, Crop section syntax, Crop, Crop @subsection Crop modes In order to be comprehensive, intuitive, and easy to use, there are two ways to define the crop: @enumerate @item From its center and side length. For example if you already know the coordinates of an object and want to inspect it in an image or to generate postage stamps of a catalog containing many such coordinates. @item The vertices of the crop region, this can be useful for larger crops over many targets, for example to crop out a uniformly deep, or contiguous, region of a large survey. @end enumerate Irrespective of how the crop region is defined, the coordinates to define the crop can be in Image (pixel) or World Coordinate System (WCS) standards. All coordinates are read as floating point numbers (not integers, except for the @option{--section} option, see below). By setting the @emph{mode} in Crop, you define the standard that the given coordinates must be interpretted. Here, the different ways to specify the crop region are discussed within each standard. For the full list options, please see @ref{Invoking astcrop}. When the crop is defined by its center, the respective (integer) central pixel position will be found internally according to the FITS standard. To have this pixel positioned in the center of the cropped region, the final cropped region will have an add number of pixels (even if you give an even number to @option{--width} in image mode). Furthermore, when the crop is defined as by its center, Crop allows you to only keep crops what don't have any blank pixels in the vicinity of their center (your primary target). This can be very convenient when your input catalog/coordinates originated from another survey/filter which is not fully covered by your input image, to learn more about this feature, please see the description of the @option{--checkcenter} option in @ref{Invoking astcrop}. @table @asis @item Image coordinates In image mode (@option{--mode=img}), Crop interprets the pixel coordinates and widths in units of the input data-elements (for example pixels in an image, not world coordinates). In image mode, only one image may be input. The output crop(s) can be defined in multiple ways as listed below. @table @asis @item Center of multiple crops (in a catalog) The center of (possibly multiple) crops are read from a text file. In this mode, the columns identified with the @option{--coordcol} option are interpreted as the center of a crop with a width of @option{--width} pixels along each dimension. The columns can contain any floating point value. The value to @option{--output} option is seen as a directory which will host (the possibly multiple) separate crop files, see @ref{Crop output} for more. For a tutorial using this feature, please see @ref{Hubble visually checks and classifies his catalog}. @item Center of a single crop (on the command-line) The center of the crop is given on the command-line with the @option{--center} option. The crop width is specified by the @option{--width} option along each dimension. The given coordinates and width can be any floating point number. @item Vertices of a single crop In Image mode there are two options to define the vertices of a region to crop: @option{--section} and @option{--polygon}. The former is lower-level (doesn't accept floating point vertices, and only a rectangular region can be defined), it is also only available in Image mode. Please see @ref{Crop section syntax} for a full description of this method. The latter option (@option{--polygon}) is a higher-level method to define any convex polygon (with any number of vertices) with floating point values. Please see the description of this option in @ref{Invoking astcrop} for its syntax. @end table @item WCS coordinates In WCS mode (@option{--mode=wcs}), the coordinates and widths are interpretted using the World Coordinate System (WCS, that must accompany the dataset), not pixel coordinates. In WCS mode, Crop accepts multiple datasets as input. When the cropped region (defined by its center or vertices) overlaps with multiple of the input images/tiles, the overlapping regions will be taken from the respective input (they will be stitched when necessary for each output crop). In this mode, the input images do not necessarily have to be the same size, they just need to have the same orientation and pixel resolution. Currently only orientation along the celestial coordinates is accepted, if your input has a different orientation you can use Warp's @option{--align} option to align the image before cropping it (see @ref{Warp}). Each individual input image/tile can even be smaller than the final crop. In any case, any part of any of the input images which overlaps with the desired region will be used in the crop. Note that if there is an overlap in the input images/tiles, the pixels from the last input image read are going to be used for the overlap. Crop will not change pixel values, so it assumes your overlapping tiles were cutout from the same original image. There are multiple ways to define your cropped region as listed below. @table @asis @item Center of multiple crops (in a catalog) Similar to catalog inputs in Image mode (above), except that the values along each dimension are assumed to have the same units as the dataset's WCS information. For example, the central RA and Dec value for each crop will be read from the first and second calls to the @option{--coordcol} option. The width of the cropped box (in units of the WCS, or degrees in RA and Dec mode) must be specified with the @option{--width} option. @item Center of a single crop (on the command-line) You can specify the center of only one crop box with the @option{--center} option. If it exists in the input images, it will be cropped similar to the catalog mode, see above also for @code{--width}. @item Vertices of a single crop The @option{--polygon} option is a high-level method to define any convex polygon (with any number of vertices). Please see the description of this option in @ref{Invoking astcrop} for its syntax. @end table @cartouche @noindent @strong{CAUTION:} In WCS mode, the image has to be aligned with the celestial coordinates, such that the first FITS axis is parallel (opposite direction) to the Right Ascension (RA) and the second FITS axis is parallel to the declination. If these conditions aren't met for an image, Crop will warn you and abort. You can use Warp's @option{--align} option to align the input image with these coordinates, see @ref{Warp}. @end cartouche @end table As a summary, if you don't specify a catalog, you have to define the cropped region manually on the command-line. In any case the mode is mandatory for Crop to be able to interpret the values given as coordinates or widths. @node Crop section syntax, Blank pixels, Crop modes, Crop @subsection Crop section syntax @cindex Crop a given section of image When in image mode, one of the methods to crop only one rectangular section from the input image is to use the @option{--section} option. Crop has a powerful syntax to read the box parameters from a string of characters. If you leave certain parts of the string to be empty, Crop can fill them for you based on the input image sizes. @cindex Define section to crop To define a box, you need the coordinates of two points: the first (@code{X1}, @code{Y1}) and the last pixel (@code{X2}, @code{Y2}) pixel positions in the image, or four integer numbers in total. The four coordinates can be specified with one string in this format: `@command{X1:X2,Y1:Y2}'. This string is given to the @option{--section} option. Therefore, the pixels along the first axis that are @mymath{\geq}@command{X1} and @mymath{\leq}@command{X2} will be included in the cropped image. The same goes for the second axis. Note that each different term will be read as an integer, not a float. This is a low-level option, for a higher-level way to specify region (any polygon, not just a box), please see the @option{--polygon} option in @ref{Crop options}. Also note that in the FITS standard, pixel indexes along each axis start from unity(1) not zero(0). @cindex Crop section format You can omit any of the values and they will be filled automatically. The left hand side of the colon (@command{:}) will be filled with @command{1}, and the right side with the image size. So, @command{2:,:} will include the full range of pixels along the second axis and only those with a first axis index larger than @command{2} in the first axis. If the colon is omitted for a dimension, then the full range is automatically used. So the same string is also equal to @command{2:,} or @command{2:} or even @command{2}. If you want such a case for the second axis, you should set it to: @command{,2}. If you specify a negative value, it will be seen as before the indexes of the image which are outside the image along the bottom or left sides when viewed in SAO ds9. In case you want to count from the top or right sides of the image, you can use an asterisk (@option{*}). When confronted with a @option{*}, Crop will replace it with the maximum length of the image in that dimension. So @command{*-10:*+10,*-20:*+20} will mean that the crop box will be @math{20\times40} pixels in size and only include the top corner of the input image with 3/4 of the image being covered by blank pixels, see @ref{Blank pixels}. If you feel more comfortable with space characters between the values, you can use as many space characters as you wish, just be careful to put your value in double quotes, for example @command{--section="5:200, 123:854"}. If you forget the quotes, anything after the first space will not be seen by @option{--section} and you will most probably get an error because the rest of your string will be read as a filename (which most probably doesn't exist). See @ref{Command-line} for a description of how the command-line works. @node Blank pixels, Invoking astcrop, Crop section syntax, Crop @subsection Blank pixels @cindex Blank pixel The cropped box can potentially include pixels that are beyond the image range. For example when a target in the input catalog was very near the edge of the input image. The parts of the cropped image that were not in the input image will be filled with the following two values depending on the data type of the image. In both cases, SAO ds9 will not color code those pixels. @itemize @item If the data type of the image is a floating point type (float or double), IEEE NaN (Not a number) will be used. @item For integer types, pixels out of the image will be filled with the value of the @command{BLANK} keyword in the cropped image header. The value assigned to it is the lowest value possible for that type, so you will probably never need it any way. Only for the unsigned character type (@command{BITPIX=8} in the FITS header), the maximum value is used because it is unsigned, the smallest value is zero which is often meaningful. @end itemize You can ask for such blank regions to not be included in the output crop image using the @option{--noblank} option. In such cases, there is no guarantee that the image size of your outputs are what you asked for. In some survey images, unfortunately they do not use the @command{BLANK} FITS keyword. Instead they just give all pixels outside of the survey area a value of zero. So by default, when dealing with float or double image types, any values that are 0.0 are also regarded as blank regions. This can be turned off with the @option{--zeroisnotblank} option. @node Invoking astcrop, , Blank pixels, Crop @subsection Invoking Crop Crop will crop a region from an image. If in WCS mode, it will also stitch parts from separate images in the input files. The executable name is @file{astcrop} with the following general template @example $ astcrop [OPTION...] [ASCIIcatalog] ASTRdata ... @end example @noindent One line examples: @example ## Crop all objects in cat.txt from image.fits: $ astcrop --catalog=cat.txt image.fits ## Crop all options in catalog (with RA,DEC) from all the files ## ending in `_drz.fits' in `/mnt/data/COSMOS/': $ astcrop --mode=wcs --catalog=cat.txt /mnt/data/COSMOS/*_drz.fits ## Crop the outer 10 border pixels of the input image: $ astcrop --section=10:*-10,10:*-10 --hdu=2 image.fits ## Crop region around RA and Dec of (189.16704, 62.218203): $ astcrop --mode=wcs --center=189.16704,62.218203 goodsnorth.fits ## Crop region around pixel coordinate (568.342, 2091.719): $ astcrop --mode=img --center=568.342,2091.719 --width=201 image.fits @end example @noindent Crop has one mandatory argument which is the input image name(s), shown above with @file{ASTRdata ...}. You can use shell expansions, for example @command{*} for this if you have lots of images in WCS mode. If the crop box centers are in a catalog, you can use the @option{--catalog} option. In other cases, you have to provide the single cropped output parameters must be given with command-line options. See @ref{Crop output} for how the output file name(s) can be specified. For the full list of general options to all Gnuastro programs (including Crop), please see @ref{Common options}. Floating point numbers can be used to specify the crop region (except the @option{--section} option, see @ref{Crop section syntax}). In such cases, the floating point values will be used to find the desired integer pixel indices based on the FITS standard. Hence, Crop ultimately doesn't do any sub-pixel cropping (in other words, it doesn't change pixel values). If you need such crops, you can use @ref{Warp} to first warp the image to the a new pixel grid, then crop from that. For example, let's assume you want a crop from pixels 12.982 to 80.982 along the first dimension. You should first translate the image by @mymath{-0.482} (note that the edge of a pixel is at integer multiples of @mymath{0.5}). So you should run Warp with @option{--translate=-0.482,0} and then crop the warped image with @option{--section=13:81}. There are two ways to define the cropped region: with its center or its vertices. See @ref{Crop modes} for a full description. In the former case, Crop can check if the central region of the cropped image is indeed filled with data or is blank (see @ref{Blank pixels}), and not produce any output when the center is blank, see the description under @option{--checkcenter} for more. @cindex Asynchronous thread allocation When in catalog mode, Crop will run in parallel unless you set @option{--numthreads=1}, see @ref{Multi-threaded operations}. Note that when multiple outputs are created with threads, the outputs will not be created in the same order. This is because the threads are asynchronous and thus not started in order. This has no effect on each output, see @ref{Hubble visually checks and classifies his catalog} for a tutorial on effectively using this feature. @menu * Crop options:: A list of all the options with explanation. * Crop output:: The outputs of Crop. @end menu @node Crop options, Crop output, Invoking astcrop, Invoking astcrop @subsubsection Crop options The options can be classified into the following contexts: Input, Output and operating mode options. Options that are common to all Gnuastro program are listed in @ref{Common options} and will not be repeated here. When you are specifying the crop vertices your self (through @option{--section}, or @option{--polygon}) on relatively small regions (depending on the resolution of your images) the outputs from image and WCS mode can be approximately equivalent. However, as the crop sizes get large, the curved nature of the WCS coordinates have to be considered. For example, when using @option{--section}, the right ascension of the bottom left and top left corners will not be equal. If you only want regions within a given right ascension, use @option{--polygon} in WCS mode. @noindent Input image parameters: @table @option @item --hstartwcs=INT Specify the first keyword card (line number) to start finding the input image world coordinate system information. Distortions were only recently included in WCSLIB (from version 5). Therefore until now, different telescope would apply their own specific set of WCS keywords and put them into the image header along with those that WCSLIB does recognize. So now that WCSLIB recognizes most of the standard distortion parameters, they will get confused with the old ones and give completely wrong results. For example in the CANDELS-GOODS South images@footnote{@url{https://archive.stsci.edu/pub/hlsp/candels/goods-s/gs-tot/v1.0/}}. The two @option{--hstartwcs} and @option{--hendwcs} are thus provided so when using older datasets, you can specify what region in the FITS headers you want to use to read the WCS keywords. Note that this is only relevant for reading the WCS information, basic data information like the image size are read separately. These two options will only be considered when the value to @option{--hendwcs} is larger than that of @option{--hstartwcs}. So if they are equal or @option{--hstartwcs} is larger than @option{--hendwcs}, then all the input keywords will be parsed to get the WCS information of the image. @item --hendwcs=INT Specify the last keyword card to read for specifying the image world coordinate system on the input images. See @option{--hstartwcs} @end table @noindent Crop box parameters: @table @option @item -c FLT[,FLT[,...]] @itemx --center=FLT[,FLT[,...]] The central position of the crop in the input image. The positions along each dimension must be separated by a comma (@key{,}) and fractions are also acceptable. The number of values given to this option must be the same as the dimensions of the input dataset. The width of the crop should be set with @code{--width}. The units of the coordinates are read based on the value to the @option{--mode} option, see below. @item -w FLT[,FLT[,...]] @itemx --width=FLT[,FLT[,...]] Width of the cropped region about its center. @option{--width} may take either a single value (to be used for all dimensions) or multiple values (a specific value for each dimension). If in WCS mode, value(s) given to this option will be read in the same units as the dataset's WCS information along this dimension. The final output will have an odd number of pixels to allow easy identification of the pixel which keeps your requested coordinate (from @option{--center} or @option{--catalog}). The @code{--width} option also accepts fractions. For example if you want the width of your crop to be 3 by 5 arcseconds along RA and Dec respectively, you can call it with: @option{--width=3/3600,5/3600}. If you want an even sided crop, you can run Crop afterwards with @option{--section=":*-1,:*-1"} or @option{--section=2:,2:} (depending on which side you don't need), see @ref{Crop section syntax}. @item -l STR @itemx --polygon=STR String of crop polygon vertices. Note that currently only convex polygons should be used. In the future we will make it work for all kinds of polygons. Convex polygons are polygons that do not have an internal angle more than 180 degrees. This option can be used both in the image and WCS modes, see @ref{Crop modes}. The cropped image will be the size of the rectangular region that completely encompasses the polygon. By default all the pixels that are outside of the polygon will be set as blank values (see @ref{Blank pixels}). However, if @option{--outpolygon} is called all pixels internal to the vertices will be set to blank. The syntax for the polygon vertices is similar to, and simpler than, that for @option{--section}. In short, the dimensions of each coordinate are separated by a comma (@key{,}) and each vertex is separated by a colon (@key{:}). You can define as many vertices as you like. If you would like to use space characters between the dimensions and vertices to make them more human-readable, then you have to put the value to this option in double quotation marks. For example, let's assume you want to work on the deepest part of the WFC3/IR images of Hubble Space Telescope eXtreme Deep Field (HST-XDF). @url{https://archive.stsci.edu/prepds/xdf/, According to the webpage}@footnote{@url{https://archive.stsci.edu/prepds/xdf/}} the deepest part is contained within the coordinates: @example [ (53.187414,-27.779152), (53.159507,-27.759633), (53.134517,-27.787144), (53.161906,-27.807208) ] @end example They have provided mask images with only these pixels in the WFC3/IR images, but what if you also need to work on the same region in the full resolution ACS images? Also what if you want to use the CANDELS data for the shallow region? Running Crop with @option{--polygon} will easily pull out this region of the image for you irrespective of the resolution. If you have set the operating mode to WCS mode in your nearest configuration file (see @ref{Configuration files}), there is no need to call @option{--mode=wcs} on the command line. You may also provide many FITS images/tiles and Crop will stitch them to produce this cropped region: @example $ astcrop --mode=wcs desired-filter-image(s).fits \ --polygon="53.187414,-27.779152 : 53.159507,-27.759633 : \ 53.134517,-27.787144 : 53.161906,-27.807208" @end example @cindex SAO ds9 In other cases, you have an image and want to define the polygon yourself (it isn't already published like the example above). As the number of vertices increases, checking the vertex coordinates on a FITS viewer (for example SAO ds9) and typing them in one by one can be very tedious and prone to typo errors. You can take the following steps to avoid the frustration and possible typos: Open the image with ds9 and activate its ``region'' mode with @clicksequence{Edit@click{}Region}. Then define the region as a polygon with @clicksequence{Region@click{}Shape@click{}Polygon}. Click on the approximate center of the region you want and a small square will appear. By clicking on the vertices of the square you can shrink or expand it, clicking and dragging anywhere on the edges will enable you to define a new vertex. After the region has been nicely defined, save it as a file with @clicksequence{Region@click{}Save Regions}. You can then select the name and address of the output file, keep the format as @command{REG} and press ``OK''. In the next window, keep format as ``ds9'' and ``Coordinate System'' as ``fk5''. A plain text file (let's call it @file{ds9.reg}) is now created. You can now convert this plain text file to Crop's polygon format with this command (when typing on the command-line, ignore the ``@key{\}'' at the end of the first and second lines along with the extra spaces, these are only for nice printing): @example $ v=$(awk 'NR==4' ds9.reg | sed -e's/polygon(//' \ -e's/\([^,]*,[^,]*\),/\1:/g' -e's/)//' ) $ astcrop --mode=wcs image.fits --polygon=$v @end example @item --outpolygon Keep all the regions outside the polygon and mask the inner ones with blank pixels (see @ref{Blank pixels}). This is practically the inverse of the default mode of treating polygons. Note that this option only works when you have only provided one input image. If multiple images are given (in WCS mode), then the full area covered by all the images has to be shown and the polygon excluded. This can lead to a very large area if large surveys like COSMOS are used. So Crop will abort and notify you. In such cases, it is best to crop out the larger region you want, then mask the smaller region with this option. @item -s STR @itemx --section=STR Section of the input image which you want to be cropped. See @ref{Crop section syntax} for a complete explanation on the syntax required for this input. @item -x STR/INT @itemx --coordcol=STR/INT The column in a catalog to read as a coordinate. The value can be either the column number (starting from 1), or a match/search in the table meta-data, see @ref{Selecting table columns}. This option must be called multiple times, depending on the number of dimensions in the input dataset. If it is called more than necessary, the extra columns (later calls to this option on the command-line or configuration files) will be ignored, see @ref{Configuration file precedence}. @item -n STR/INT @item --namecol=STR/INT Column selection of crop file name. The value can be either the column number (starting from 1), or a match/search in the table meta-data, see @ref{Selecting table columns}. This option can be used both in Image and WCS modes, and not a mandatory. When a column is given to this option, the final crop base file name will be taken from the contents of this column. The directory will be determined by the @option{--output} option (current directory if not given) and the value to @option{--suffix} will be appended. When this column isn't given, the row number will be used instead. @end table @noindent Output options: @table @option @item -c INT @itemx --checkcenter=INT @cindex Check center of crop Box width (odd number of pixels) of region in the center of the image to check for blank values. If the value to this option is zero, no checking is done. This option is only relevant when the cropped region(s) are defined by their center (not by the vertices, see @ref{Crop modes}). If any of the pixels in this central region of a crop (defined by its center) are blank, then it will not be created. Because survey regions don't often have a clean square or rectangle shape, some of the pixels on the sides of the survey FITS image don't commonly have any data and are blank (see @ref{Blank pixels}). So when the catalog was not generated from the input image, it often happens that the image does not have data over some of the points. When the given center of a crop falls in such regions and this option has a non-zero, odd value, no crop will be created. Therefore with this option, you can specify a width of a small box (3 pixels is often good enough) around the central pixel of the cropped image. You can check which crops were created and which weren't from the command-line (if @option{--quiet} was not called, see @ref{Operating mode options}), or in Crop's log file (see @ref{Crop output}). @item -p STR @itemx --suffix=STR The suffix (or post-fix) of the output files for when you want all the cropped images to have a special ending. One case where this might be helpful is when besides the science images, you want the weight images (or exposure maps, which are also distributed with survey images) of the cropped regions too. So in one run, you can set the input images to the science images and @option{--suffix=_s.fits}. In the next run you can set the weight images as input and @option{--suffix=_w.fits}. @item -b @itemx --noblank Pixels outside of the input image that are in the crop box will not be used. By default they are filled with blank values (depending on type), see @ref{Blank pixels}. This option only applies only in Image mode, see @ref{Crop modes}. @item -z @itemx --zeroisnotblank In float or double images, it is common to give the value of zero to blank pixels. If the input image type is one of these two types, such pixels will also be considered as blank. You can disable this behavior with this option, see @ref{Blank pixels}. @end table @noindent Operating mode options: @table @option @item -O STR @itemx --mode=STR Operate in Image mode or WCS mode when the input coordinates can be both image or WCS. The value must either be @option{img} or @option{wcs}, see @ref{Crop modes} for a full description. @end table @node Crop output, , Crop options, Invoking astcrop @subsubsection Crop output The string given to @option{--output} option will be interpretted depending on how many crops were requested, see @ref{Crop modes}: @itemize @item When a catalog is given, the value of the @option{--output} (see @ref{Common options}) will be read as the directory to store the output cropped images. Hence if it doesn't already exist, Crop will abort with an error of a ``No such file or directory'' error. The crop file names will consist of two parts: a variable part (the row number of each target starting from 1) along with a fixed string which you can set with the @option{--suffix} option. Optionally, you may also use the @option{--namecol} option to define a column in the input catalog to use as the file name instead of numbers. @item When only one crop is desired, the value to @option{--output} will be read as a file name. If no output is specified or if it is a directory, the output file name will follow the automatic output names of Gnuastro, see @ref{Automatic output}: The string given to @option{--suffix} will be replaced with the @file{.fits} suffix of the input. @end itemize The header of each output cropped image will contain the names of the input image(s) it was cut from. If a name is longer than the 70 character space that the FITS standard allows for header keyword values, the name will be cut into several keywords from the nearest slash (@key{/}). The keywords have the following format: @command{ICFn_m} (for Crop File). Where @command{n} is the number of the image used in this crop and @command{m} is the part of the name (it can be broken into multiple keywords). Following the name is another keyword named @command{ICFnPIX} which shows the pixel range from that input image in the same syntax as @ref{Crop section syntax}. So this string can be directly given to the @option{--section} option later. Once done, a log file can be created in the current directory with the @code{--log} option. This file will have three columns and the same number of rows as the number of cropped images. There are also comments on the top of the log file explaining basic information about the run and descriptions for the columns. A short description of the columns is also given below: @enumerate @item The cropped image file name for that row. @item The number of input images that were used to create that image. @item A @code{0} if the central few pixels (value to the @option{--checkcenter} option) are blank and @code{1} if they aren't. When the crop was not defined by its center (see @ref{Crop modes}), or @option{--checkcenter} was given a value of 0 (see @ref{Invoking astcrop}), the center will not be checked and this column will be given a value of @code{-1}. @end enumerate @node Arithmetic, Convolve, Crop, Data manipulation @section Arithmetic It is commonly necessary to do operations on some or all of the elements of a dataset independently (pixels in an image). For example, in the reduction of raw data it is necessary to subtract the Sky value (@ref{Sky value}) from each image image. Later (once the images as warped into a single grid using Warp for example, see @ref{Warp}), the images are co-added (the output pixel grid is the average of the pixels of the individual input images). Arithmetic is Gnuastro's program for such operations on your datasets directly from the command-line. It currently uses the reverse polish or post-fix notation, see @ref{Reverse polish notation} and will work on the native data types of the input images/data to reduce CPU and RAM resources, see @ref{Numeric data types}. For more information on how to run Arithmetic, please see @ref{Invoking astarithmetic}. @menu * Reverse polish notation:: The current notation style for Arithmetic * Arithmetic operators:: List of operators known to Arithmetic * Invoking astarithmetic:: How to run Arithmetic: options and output @end menu @node Reverse polish notation, Arithmetic operators, Arithmetic, Arithmetic @subsection Reverse polish notation @cindex Post-fix notation @cindex Reverse Polish Notation The most common notation for arithmetic operations is the @url{https://en.wikipedia.org/wiki/Infix_notation, infix notation} where the operator goes between the two operands, for example @mymath{4+5}. While the infix notation is the preferred way in most programming languages, currently Arithmetic does not use it since it will require parenthesis which can complicate the implementation of the code. In the near future we do plan to adopt this notation@footnote{@url{https://savannah.gnu.org/task/index.php?13867}}, but for the time being (due to time constraints on the developers), Arithmetic uses the post-fix or @url{https://en.wikipedia.org/wiki/Reverse_Polish_notation, reverse polish notation}. The Wikipedia article provides some excellent explanation on this notation but here we will give a short summary here for self-sufficiency. In the post-fix notation, the operator is placed after the operands, as we will see below this removes the need to define parenthesis for most ordinary operators. For example, instead of writing @command{5+6}, we write @command{5 6 +}. To easily understand how this notation works, you can think of each operand as a node in a first-in-first-out stack. Every time an operator is confronted, it pops the number of operands it needs from the top of the stack (so they don't exist in the stack any more), does its operation and pushes the result back on top of the stack. So if you want the average of 5 and 6, you would write: @command{5 6 + 2 /}. The operations that are done are: @enumerate @item @command{5} is an operand, so it is pushed to the top of the stack. @item @command{6} is an operand, so it is pushed to the top of the stack. @item @command{+} is a binary operator, so pull the top two elements of the stack and perform addition on them (the order is @mymath{5+6} in the example above). The result is @command{11}, push it on top of the stack. @item @command{2} is an operand so push it onto the top of the stack. @item @command{/} is a binary operator, so pull out the top two elements of the stack (top-most is @command{2}, then @command{11}) and divide the second one by the first. @end enumerate In the Arithmetic program, the operands can be FITS images or numbers. As you can see, very complicated procedures can be created without the need for parenthesis or worrying about precedence. Even functions which take an arbitrary number of arguments can be defined in this notation. This is a very powerful notation and is used in languages like Postscript @footnote{See the EPS and PDF part of @ref{Recognized file formats} for a little more on the Postscript language.} (the programming language in Postscript and compiled into PDF files) uses this notation. @node Arithmetic operators, Invoking astarithmetic, Reverse polish notation, Arithmetic @subsection Arithmetic operators The recognized operators in Arithmetic are listed below. See @ref{Reverse polish notation} for more on how the operators and operands should be ordered on the command-line. The operands to all operators can be a data array (for example a FITS image) or a number, the output will be an array or number according to the inputs. For example a number multiplied by an array will produce an array. The conditional operators will return pixel, or numerical values of 0 (false) or 1 (true) and stored in an @code{unsigned char} data type (see @ref{Numeric data types}). @table @command @item + Addition, so ``@command{4 5 +}'' is equivalent to @mymath{4+5}. @item - Subtraction, so ``@command{4 5 -}'' is equivalent to @mymath{4-5}. @item x Multiplication, so ``@command{4 5 x}'' is equivalent to @mymath{4\times5}. @item / Division, so ``@command{4 5 /}'' is equivalent to @mymath{4/5}. @item % Modulo (remainder), so ``@command{3 2 %}'' is equivalent to @mymath{1}. Note that the modulo operator only works on integer types. @item abs Absolute value of first operand, so ``@command{4 abs}'' is equivalent to @mymath{|4|}. @item pow First operand to the power of the second, so ``@command{4.3 5f pow}'' is equivalent to @mymath{4.3^{5}}. Currently @code{pow} will only work on single or double precision floating point numbers or images. To be sure that a number is read as a floating point (even if it doesn't have any non-zero decimals) put an @code{f} after it. @item sqrt The square root of the first operand, so ``@command{5 sqrt}'' is equivalent to @mymath{\sqrt{5}}. The output type is determined from the input, so the output of this example will be @command{2} (since @command{5} doesn't have any non-zero decimal digits). If you want @command{2.23607}, run @command{5f sqrt} instead, the @command{f} will ensure that a number will be read as a floating point number, even if it doesn't have decimal digits. If the input image has an integer type, you should explicitly convert the image to floating point, for example @command{a.fits float sqrt}, see the type conversion operators below. @item log Natural logarithm of first operand, so ``@command{4 log}'' is equivalent to @mymath{\ln(4)}. The output type is determined from the input, see the explanation under @command{sqrt} for more. @item log10 Base-10 logarithm of first operand, so ``@command{4 log10}'' is equivalent to @mymath{\log(4)}. The output type is determined from the input, see the explanation under @command{sqrt} for more. @item minvalue Minimum (non-blank) value in the top operand on the stack, so ``@command{a.fits minvalue}'' will push the the minimum pixel value in this image onto the stack. Therefore this operator is mainly intended for data (for example images), if the top operand is a number, this operator just returns it without any change. So note that when this operator acts on a single image, the output will no longer be an image, but a number. The output of this operand is in the same type as the input. @item maxvalue Maximum (non-blank) value of first operand in the same type, similar to @command{minvalue}. @item numvalue Number of non-blank elements in first operand in the @code{uint64} type, similar to @command{minvalue}. @item sumvalue Sum of non-blank elements in first operand in the @code{float32} type, similar to @command{minvalue}. @item meanvalue Mean value of non-blank elements in first operand in the @code{float32} type, similar to @command{minvalue}. @item stdvalue Standard deviation of non-blank elements in first operand in the @code{float32} type, similar to @command{minvalue}. @item medianvalue Median of non-blank elements in first operand with the same type, similar to @command{minvalue}. @cindex NaN @item min The first popped operand to this operator must be a positive integer number which specifies how many further operands should be popped from the stack. The given number of operands must have the same type and size. Each pixel of the output of this operator will be set to the minimum value of the given number of operands (images) in that pixel. For example the following command will produce an image with the same size and type as the inputs but each output pixel is set to the minimum respective pixel value of the three input images. @example $ astarithmetic a.fits b.fits c.fits 3 min @end example Important notes: @itemize @item NaN/blank pixels will be ignored, see @ref{Blank pixels}. @item The output will have the same type as the inputs. This is natural for the @command{min} and @command{max} operators, but for other similar operators (for example @command{sum}, or @command{average}) the per-pixel operations will be done in double precision floating point and then stored back in the input type. Therefore, if the input was an integer, C's internal type conversion will be used. @end itemize @item max Similar to @command{min}, but the pixels of the output will contain the maximum of the respective pixels in all operands in the stack. @item num Similar to @command{min}, but the pixels of the output will contain the number of the respective non-blank pixels in all input operands. @item sum Similar to @command{min}, but the pixels of the output will contain the sum of the respective pixels in all input operands. @item mean Similar to @command{min}, but the pixels of the output will contain the mean (average) of the respective pixels in all operands in the stack. @item std Similar to @command{min}, but the pixels of the output will contain the standard deviation of the respective pixels in all operands in the stack. @item median Similar to @command{min}, but the pixels of the output will contain the median of the respective pixels in all operands in the stack. @item filter-mean Apply mean filtering (or @url{https://en.wikipedia.org/wiki/Moving_average, moving average}) on the input dataset. During mean filtering, each pixel (data element) is replaced by the mean value of all its surrounding pixels (excluding blank values). The number of surrounding pixels in each dimension (to calculate the mean) is determined through the earlier operands that have been pushed onto the stack prior to the input dataset. The number of necessary operands is determined by the dimensions of the input dataset (first popped operand). The order of the dimensions on the command-line is the order in FITS format. Here is one example: @example $ astarithmetic 5 4 image.fits filter-mean @end example @noindent In this example, each pixel is replaced by the mean of a 5 by 4 box around it. The box is 5 pixels along the first FITS dimension (horizontal when viewed in ds9) and 4 pixels along the second FITS dimension (vertical). Each pixel will be placed in the center of the box that the mean is calculated on. If the given width along a dimension is even, then the center is assumed to be between the pixels (not in the center of a pixel). When the pixel is close to the center, the pixels of the box that fall outside the image are ignored. Therefore, on the edge, less points will be used in calculating the mean. The final effect of mean filtering is to smooth the input image, it is essentially a convolution with a kernel that has identical values for all its pixels (is flat), see @ref{Convolution process}. @item filter-median Apply @url{https://en.wikipedia.org/wiki/Median_filter, median filtering} on the input dataset. This is very similar to @command{filter-mean}, except that instead of the mean value of the box pixels, the median value is used to replace a pixel value. For more on how to use this operator, please see @command{filter-mean}. The median is less susceptible to outliers compared to the mean. As a result, after median filtering, the pixel values will be more discontinuous than mean filtering. @item lt Less than: If the second popped (or left operand in infix notation, see @ref{Reverse polish notation}) value is smaller than the first popped operand, then this function will return a value of 1, otherwise it will return a value of 0. If both operands are images, then all the pixels will be compared with their counterparts in the other image. If only one operand is an image, then all the pixels will be compared with the the single value (number) of the other operand. Finally if both are numbers, then the output is also just one number (0 or 1). When the output is not a single number, it will be stored as an @code{unsigned char} type. @item le Less or equal: similar to @code{lt} (`less than' operator), but returning 1 when the second popped operand is smaller or equal to the first. @item gt Greater than: similar to @code{lt} (`less than' operator), but returning 1 when the second popped operand is greater than the first. @item ge Greater or equal: similar to @code{lt} (`less than' operator), but returning 1 when the second popped operand is larger or equal to the first. @item eq Equality: similar to @code{lt} (`less than' operator), but returning 1 when the two popped operands are equal (to double precision floating point accuracy). @item ne Non-Equality: similar to @code{lt} (`less than' operator), but returning 1 when the two popped operands are @emph{not} equal (to double precision floating point accuracy). @item and Logical AND: returns 1 if both operands have a non-zero value and 0 if both are zero. Both operands have to be the same kind: either both images or both numbers. @item or Logical OR: returns 1 if either one of the operands is non-zero and 0 only when both operators are zero. Both operands have to be the same kind: either both images or both numbers. @item not Logical NOT: returns 1 when the operand is zero and 0 when the operand is non-zero. The operand can be an image or number, for an image, it is applied to each pixel separately. @cindex Blank pixel @item isblank Test for a blank value (see @ref{Blank pixels}). In essence, this is very similar to the conditional operators: the output is either 1 or 0 (see the `less than' operator above). The difference is that it only needs one operand. Because of the definition of a blank pixel, a blank value is not even equal to itself, so you cannot use the equal operator above to select blank pixels. See the ``Blank pixels'' box below for more on Blank pixels in Arithmetic. @item where Change the input (pixel) value @emph{where}/if a certain condition holds. The conditional operators above can be used to define the condition. Three operands are required for @command{where}. The input format is demonstrated in this simplified example: @example $ astarithmetic modify.fits binary.fits if-true.fits where @end example The value of any pixel in @file{modify.fits} that corresponds to a non-zero pixel of @file{binary.fits} will be changed to the value of the same pixel in @file{if-true.fits} (this may also be a number). The 3rd and 2nd popped operands (@file{modify.fits} and @file{binary.fits} respectively, see @ref{Reverse polish notation}) have to have the same dimensions/size. @file{if-true.fits} can be either a number, or have the same dimension/size as the other two. The 2nd popped operand (@file{binary.fits}) has to have @code{uint8} (or @code{unsigned char} in standard C) type (see @ref{Numeric data types}). It is treated as a binary dataset (with only two values: zero and non-zero, hence the name @code{binary.fits} in this example). However, commonly you won't be dealing with an actual FITS file of a condition/binary image. You will probably define the condition in the same run based on some other reference image and use the conditional and logical operators above to make a true/false (or one/zero) image for you internally. For example the case below: @example $ astarithmetic in.fits reference.fits 100 gt new.fits where @end example In the example above, any of the @file{in.fits} pixels that has a value in @file{reference.fits} greater than @command{100}, will be replaced with the corresponding pixel in @file{new.fits}. Effectively the @code{reference.fits 100 gt} part created the condition/binary image which was added to the stack (in memory) and later used by @code{where}. The command above is thus equivalent to these two commands: @example $ astarithmetic reference.fits 100 gt --output=binary.fits $ astarithmetic in.fits binary.fits new.fits where @end example Finally, the input operands are read and used independently, so you can use the same file more than once as any of the operands. When the 1st popped operand to @code{where} (@file{if-true.fits}) is a single number, it may be a NaN value (or any blank value, depending on its type) like the example below (see @ref{Blank pixels}). When the number is blank, it will be converted to the blank value of the type of the 3rd popped operand (@code{in.fits}). Hence, in the example below, all the pixels in @file{reference.fits} that have a value greater than 100, will become blank in the natural data type of @file{in.fits} (even though NaN values are only defined for floating point types). @example $ astarithmetic in.fits reference.fits 100 gt nan where @end example @item bitand Bitwise AND operator: only bits with values of 1 in both popped operands will get the value of 1, the rest will be set to 0. For example (assuming numbers can be written as bit strings on the command-line): @code{00101000 00100010 bitand} will give @code{00100000}. Note that the bitwise operators only work on integer type datasets. @item bitor Bitwise inclusive OR operator: The bits where at least one of the two popped operands has a 1 value get a value of 1, the others 0. For example (assuming numbers can be written as bit strings on the command-line): @code{00101000 00100010 bitand} will give @code{00101010}. Note that the bitwise operators only work on integer type datasets. @item bitxor Bitwise exclusive OR operator: A bit will be 1 if it differs between the two popped operands. For example (assuming numbers can be written as bit strings on the command-line): @code{00101000 00100010 bitand} will give @code{00001010}. Note that the bitwise operators only work on integer type datasets. @item lshift Bitwise left shift operator: shift all the bits of the first operand to the left by a number of times given by the second operand. For example (assuming numbers can be written as bit strings on the command-line): @code{00101000 2 lshift} will give @code{10100000}. This is equivalent to multiplication by 4. Note that the bitwise operators only work on integer type datasets. @item rshift Bitwise right shift operator: shift all the bits of the first operand to the right by a number of times given by the second operand. For example (assuming numbers can be written as bit strings on the command-line): @code{00101000 2 rshift} will give @code{00001010}. Note that the bitwise operators only work on integer type datasets. @item bitnot Bitwise not (more formally known as one's complement) operator: flip all the bits of the popped operand (note that this is the only unary, or single operand, bitwise operator). In other words, any bit with a value of @code{0} is changed to @code{1} and vice-versa. For example (assuming numbers can be written as bit strings on the command-line): @code{00101000 bitnot} will give @code{11010111}. Note that the bitwise operators only work on integer type datasets/numbers. @item uint8 Convert the type of the popped operand to 8-bit un-signed integer type (see @ref{Numeric data types}). The internal conversion of C will be used. @item int8 Convert the type of the popped operand to 8-bit signed integer type (see @ref{Numeric data types}). The internal conversion of C will be used. @item uint16 Convert the type of the popped operand to 16-bit un-signed integer type (see @ref{Numeric data types}). The internal conversion of C will be used. @item int16 Convert the type of the popped operand to 16-bit signed integer (see @ref{Numeric data types}). The internal conversion of C will be used. @item uint32 Convert the type of the popped operand to 32-bit un-signed integer type (see @ref{Numeric data types}). The internal conversion of C will be used. @item int32 Convert the type of the popped operand to 32-bit signed integer type (see @ref{Numeric data types}). The internal conversion of C will be used. @item uint64 Convert the type of the popped operand to 64-bit un-signed integer (see @ref{Numeric data types}). The internal conversion of C will be used. @item float32 Convert the type of the popped operand to 32-bit (single precision) floating point (see @ref{Numeric data types}). The internal conversion of C will be used. @item float64 Convert the type of the popped operand to 64-bit (double precision) floating point (see @ref{Numeric data types}). The internal conversion of C will be used. @end table @cartouche @noindent @strong{Blank pixels in Arithmetic:} Blank pixels in the image (see @ref{Blank pixels}) will be stored based on the data type. When the input is floating point type, blank values are NaN. One aspect of NaN values is that by definition they will fail on @emph{any} comparison. Hence both equal and not-equal operators will fail when both their operands are NaN! Therefore, the only way to guarantee selection of blank pixels is through the @command{isblank} operator explained above. One way you can exploit this property of the NaN value to your advantage is when you want a fully zero-valued image (even over the blank pixels) based on an already existing image (with same size and world coordinate system settings). The following command will produce this for you: @example $ astarithmetic input.fits nan eq --output=all-zeros.fits @end example @noindent Note that on the command-line you can write NaN in any case (for example @command{NaN}, or @command{NAN} are also acceptable). Reading NaN as a floating point number in Gnuastro isn't case-sensitive. @end cartouche @node Invoking astarithmetic, , Arithmetic operators, Arithmetic @subsection Invoking Arithmetic Arithmetic will do pixel to pixel arithmetic operations on the individual pixels of input data and/or numbers. For the full list of operators with explanations, please see @ref{Arithmetic operators}. Any operand that only has a single element (number, or single pixel FITS image) will be read as a number, the rest of the inputs must have the same dimensions. The general template is: @example $ astarithmetic [OPTION...] ASTRdata1 [ASTRdata2] OPERATOR ... @end example @noindent One line examples: @example ## Calculate (10.32-3.84)^2.7 quietly (will just print 155.329): $ astarithmetic -q 10.32 3.84 - 2.7 pow ## Inverse the input image (1/pixel): $ astarithmetic 1 image.fits / --out=inverse.fits ## Multiply each pixel in image by -1: $ astarithmetic image.fits -1 x --out=negative.fits ## Subtract extension 4 from extension 1 (counting from zero): $ astarithmetic image.fits image.fits - --out=skysub.fits \ --hdu=1 --hdu=4 ## Add two images, then divide them by 2 (2 is read as floating point): $ astarithmetic image1.fits image2.fits + 2f / --out=average.fits ## Use Arithmetic's average operator: $ astarithmetic image1.fits image2.fits average --out=average.fits ## Calculate the median of three images in three separate extensions: $ astarithmetic img1.fits img2.fits img3.fits median \ -h0 -h1 -h2 --out=median.fits @end example If the output is an image, and the @option{--output} option is not given, automatic output will use the name of the first FITS image encountered to generate an output file name, see @ref{Automatic output}. Also, output WCS information will be taken from the first input image encountered. When the output is a single number, that number will be printed in the standard output and no output file will be created. Arithmetic's notation for giving operands to operators is described in @ref{Reverse polish notation}. To ignore certain pixels, set them as blank, see @ref{Blank pixels}, for example with the @command{where} operator (see @ref{Arithmetic operators}). See @ref{Common options} for a review of the options in all Gnuastro programs. Arithmetic just redefines the @option{--hdu} option as explained below: @table @option @item -h INT/STR @itemx --hdu INT/STR The header data unit of the input FITS images, see @ref{Input output options}. Unlike most options in Gnuastro (which will ultimately only have one value for this option), Arithmetic allows @option{--hdu} to be called multiple times and the value of each invocation will be stored separately (for the unlimited number of input images you would like to use). Recall that for other programs this (common) option only takes a single value. So in other programs, if you specify it multiple times on the command-line, only the last value will be used and in the configuration files, it will be ignored if it already has a value. The order of the values to @option{--hdu} has to be in the same order as input FITS images. Options are first read from the command-line (from left to right), then top-down in each configuration file, see @ref{Configuration file precedence}. If the number of HDUs is less than the number of input images, Arithmetic will abort and notify you. However, if there are more HDUs than FITS images, there is no problem: they will be used in the given order (every time a FITS image comes up on the stack) and the extra HDUs will be ignored in the end. So there is no problem with having extra HDUs in the configuration files and by default several HDUs with a value of @option{0} are kept in the system-wide configuration file when you install Gnuastro. @item -g INT/STR @itemx --globalhdu INT/STR Use the value to this option as the HDU of all input FITS files. This option is very convenient when you have many input files and the dataset of interest is in the same HDU of all the files. When this option is called, any values given to the @option{--hdu} option (explained above) are ignored and will not be used. @end table Arithmetic accepts two kinds of input: images and numbers. Images are considered to be any of the inputs that is a file name of a recognized type (see @ref{Arguments}) and has more than one element/pixel. Numbers on the command-line will be read into the smallest type (see @ref{Numeric data types}) that can store them, so @command{-2} will be read as a @code{char} type (which is signed on most systems and can thus keep negative values), @command{2500} will be read as an @code{unsigned short} (all positive numbers will be read as unsigned), while @code{3.1415926535897} will be read as a @code{double} and @code{3.14} will be read as a @code{float}. To force a number to be read as float, add a @code{f} after it, so @command{5f} will be added to the stack as @code{float} (see @ref{Reverse polish notation}). Unless otherwise stated (in @ref{Arithmetic operators}), the operators can deal with numeric multiple data types (see @ref{Numeric data types}). For example in ``@command{a.fits b.fits +}'', the image types can be @code{long} and @code{float}. In such cases, C's internal type conversion will be used. The output type will be set to the higher-ranking type of the two inputs. Unsigned integer types have smaller ranking than their signed counterparts and floating point types have higher ranking than the integer types. So the internal C type conversions done in the example above are equivalent to this piece of C: @example size_t i; long a[100]; float b[100], out[100]; for(i=0;i<100;++i) out[i]=a[i]+b[i]; @end example @noindent Relying on the default C type conversion significantly speeds up the processing and also requires less RAM (when using very large images). Some operators can only work on integer types (of any length, for example bitwise operators) while others only work on floating point types, (currently only the @code{pow} operator). In such cases, if the operand type(s) are different, an error will be printed. Arithmetic also comes with internal type conversion operators which you can use to convert the data into the appropriate type, see @ref{Arithmetic operators}. @cindex Options The hyphen (@command{-}) can be used both to specify options (see @ref{Options}) and also to specify a negative number which might be necessary in your arithmetic. In order to enable you to do this, Arithmetic will first parse all the input strings and if the first character after a hyphen is a digit, then that hyphen is temporarily replaced by the vertical tab character which is not commonly used. The arguments are then parsed and these strings will not be specified as an option. Then the given arguments are parsed and any vertical tabs are replaced back with a hyphen so they can be read as negative numbers. Therefore, as long as the names of the files you want to work on, don't start with a vertical tab followed by a digit, there is no problem. An important consequence of this implementation is that you should not write negative fractions like this: @command{-.3}, instead write them as @command{-0.3}. @cindex AWK @cindex GNU AWK Without any images, Arithmetic will act like a simple calculator and print the resulting output number on the standard output like the first example above. If you really want such calculator operations on the command-line, AWK (GNU AWK is the most common implementation) is much faster, easier and much more powerful. For example, the numerical one-line example above can be done with the following command. In general AWK is a fantastic tool and GNU AWK has a wonderful manual (@url{https://www.gnu.org/software/gawk/manual/}). So if you often confront situations like this, or have to work with large text tables/catalogs, be sure to checkout AWK and simplify your life. @example $ echo "" | awk '@{print (10.32-3.84)^2.7@}' 155.329 @end example @node Convolve, Warp, Arithmetic, Data manipulation @section Convolve @cindex Convolution @cindex Neighborhood @cindex Weighted average @cindex Average, weighted @cindex Kernel, convolution On an image, convolution can be thought of as a process to blur or remove the contrast in an image. If you are already familiar with the concept and just want to run Convolve, you can jump to @ref{Convolution kernel} and @ref{Invoking astconvolve} and skip the lengthy introduction on the basic definitions and concepts of convolution. There are generally two methods to convolve an image. The first and more intuitive one is in the ``spatial domain'' or using the actual image pixel values, see @ref{Spatial domain convolution}. The second method is when we manipulate the ``frequency domain'', or work on the magnitudes of the different frequencies that constitute the image, see @ref{Frequency domain and Fourier operations}. Understanding convolution in the spatial domain is more intuitive and thus recommended if you are just starting to learn about convolution. However, getting a good grasp of the frequency domain is a little more involved and needs some concentration and some mathematical proofs. However, its reward is a faster operation and more importantly a very fundamental understanding of this very important operation. @cindex Detection @cindex Atmosphere @cindex Blur image @cindex Cosmic rays @cindex Pixel mixing @cindex Mixing pixel values Convolution of an image will generally result in blurring the image because it mixes pixel values. In other words, if the image has sharp differences in neighboring pixel values@footnote{In astronomy, the only major time we confront such sharp borders in signal are cosmic rays. All other sources of signal in an image are already blurred by the atmosphere or the optics of the instrument.}, those sharp differences will become smoother. This has very good consequences in detection of signal in noise for example. In an actual observed image, the variation in neighboring pixel values due to noise can be very high. But after convolution, those variations will decrease and we have a better hope in detecting the possible underlying signal. Another case where convolution is extensively used is in mock images and modeling in general, convolution can be used to simulate the effect of the atmosphere or the optical system on the mock profiles that we create, see @ref{PSF}. Convolution is a very interesting and important topic in any form of signal analysis (including astronomical observations). So we have thoroughly@footnote{A mathematician will certainly consider this explanation is incomplete and inaccurate. However this text is written for an understanding on the operations that are done on a real (not complex, discrete and noisy) astronomical image, not any general form of abstract function} explained the concepts behind it in the following sub-sections. @menu * Spatial domain convolution:: Only using the input image values. * Frequency domain and Fourier operations:: Using frequencies in input. * Spatial vs. Frequency domain:: When to use which? * Convolution kernel:: How to specify the convolution kernel. * Invoking astconvolve:: Options and argument to Convolve. @end menu @node Spatial domain convolution, Frequency domain and Fourier operations, Convolve, Convolve @subsection Spatial domain convolution The pixels in an input image represent different ``spatial'' positions, therefore when convolution is done only using the actual input pixel values, we name the process as being done in the ``Spatial domain''. In particular this is in contrast to the ``frequency domain'' that we will discuss later in @ref{Frequency domain and Fourier operations}. In the spatial domain (and in realistic situations where the image and the convolution kernel don't extend to infinity), convolution is the process of changing the value of one pixel to the @emph{weighted} average of all the pixels in its @emph{neighborhood}. The `neighborhood' of each pixel (how many pixels in which direction) and the `weight' function (how much each neighboring pixel should contribute depending on its position) are given through a second image which is known as a ``kernel''@footnote{Also known as filter, here we will use `kernel'.}. @menu * Convolution process:: More basic explanations. * Edges in the spatial domain:: Dealing with the edges of an image. @end menu @node Convolution process, Edges in the spatial domain, Spatial domain convolution, Spatial domain convolution @subsubsection Convolution process In convolution, the kernel specifies the weight and positions of the neighbors of each pixel. To find the convolved value of a pixel, the central pixel of the kernel is placed on that pixel. The values of each overlapping pixel in the kernel and image are multiplied by each other and summed for all the kernel pixels. To have one pixel in the center, the sides of the convolution kernel have to be an odd number. This process effectively mixes the pixel values of each pixel with its neighbors, resulting in a blurred image compared to the sharper input image. @cindex Linear spatial filtering Formally, convolution is one kind of linear `spatial filtering' in image processing texts. If we assume that the kernel has @mymath{2a+1} and @mymath{2b+1} pixels on each side, the convolved value of a pixel placed at @mymath{x} and @mymath{y} (@mymath{C_{x,y}}) can be calculated from the neighboring pixel values in the input image (@mymath{I}) and the kernel (@mymath{K}) from @dispmath{C_{x,y}=\sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t}.} @cindex Correlation @cindex Convolution Any pixel coordinate that is outside of the image in the equation above will be considered to be zero. When the kernel is symmetric about its center the blurred image has the same orientation as the original image. However, if the kernel is not symmetric, the image will be affected in the opposite manner, this is a natural consequence of the definition of spatial filtering. In order to avoid this we can rotate the kernel about its center by 180 degrees so the convolved output can have the same original orientation. Technically speaking, only if the kernel is flipped the process is known @emph{Convolution}. If it isn't it is known as @emph{Correlation}. To be a weighted average, the sum of the weights (the pixels in the kernel) have to be unity. This will have the consequence that the convolved image of an object and un-convolved object will have the same brightness (see @ref{Flux Brightness and magnitude}), which is natural, because convolution should not eat up the object photons, it only disperses them. @node Edges in the spatial domain, , Convolution process, Spatial domain convolution @subsubsection Edges in the spatial domain In purely `linear' spatial filtering (convolution), there are problems on the edges of the input image. Here we will explain the problem in the spatial domain. For a discussion of this problem from the frequency domain perspective, see @ref{Edges in the frequency domain}. The problem originates from the fact that on the edges, in practice@footnote{Because we assumed the overlapping pixels outside the input image have a value of zero.}, the sum of the weights we use on the actual image pixels is not unity. For example, as discussed above, a profile in the center of an image will have the same brightness before and after convolution. However, for partially imaged profile on the edge of the image, the brightness (sum of its pixel fluxes within the image, see @ref{Flux Brightness and magnitude}) will not be equal, some of the flux is going to be `eaten' by the edges. If you ran @command{$ make check} on the source files of Gnuastro, you can see the this effect by comparing the @file{convolve_frequency.fits} with @file{convolve_spatial.fits} in the @file{./tests/} directory. In the spatial domain, by default, no assumption will be made about pixels outside of the image or any blank pixels in the image. The problem explained above will also occur on the sides of blank regions (see @ref{Blank pixels}). The solution to this edge effect problem is only possible in the spatial domain. For pixels near the edge, we have to abandon the assumption that the sum of the kernel pixels is unity during the convolution process@footnote{ofcourse the sum of the kernel pixels still have to be unity in general.}. So taking @mymath{W} as the sum of the kernel pixels that overlapped with non-blank and in-image pixels, the equation in @ref{Convolution process} will become: @dispmath{C_{x,y}= { \sum_{s=-a}^{a}\sum_{t=-b}^{b}K_{s,t}\times{}I_{x+s,y+t} \over W}.} @noindent In this manner, objects which are near the edges of the image or blank pixels will also have the same brightness (within the image) before and after convolution. This correction is applied by default in Convolve when convolving in the spatial domain. To disable it, you can use the @option{--noedgecorrection} option. In the frequency domain, there is no way to avoid this loss of flux near the edges of the image, see @ref{Edges in the frequency domain} for an interpretation from the frequency domain perspective. Note that the edge effect discussed here is different from the one in @ref{If convolving afterwards}. In making mock images we want to simulate a real observation. In a real observation the images of the galaxies on the sides of the CCD are first blurred by the atmosphere and instrument, then imaged. So light from the parts of a galaxy which are immediately outside the CCD will affect the parts of the galaxy which are covered by the CCD. Therefore in modeling the observation, we have to convolve an image that is larger than the input image by exactly half of the convolution kernel. We can hence conclude that this correction for the edges is only useful when working on actual observed images (where we don't have any more data on the edges) and not in modeling. @node Frequency domain and Fourier operations, Spatial vs. Frequency domain, Spatial domain convolution, Convolve @subsection Frequency domain and Fourier operations Getting a good grip on the frequency domain is usually not an easy job! So we have decided to give the issue a complete review here. Convolution in the frequency domain (see @ref{Convolution theorem}) heavily relies on the concepts of Fourier transform (@ref{Fourier transform}) and Fourier series (@ref{Fourier series}) so we will be investigating these important operations first. It has become something of a clich@'e for people to say that the Fourier series ``is a way to represent a (wave-like) function as the sum of simple sine waves'' (from Wikipedia). However, sines themselves are abstract functions, so this statement really adds no extra layer of physical insight. Before jumping head-first into the equations and proofs, we will begin with a historical background to see how the importance of frequencies actually roots in our ancient desire to see everything in terms of circles. A short review of how the complex plane should be interpreted is then given. Having paved the way with these two basics, we define the Fourier series and subsequently the Fourier transform. The final aim is to explain discrete Fourier transform, however some very important concepts need to be solidified first: The Dirac comb, convolution theorem and sampling theorem. So each of these topics are explained in their own separate sub-sub-section before going on to the discrete Fourier transform. Finally we revisit (after @ref{Edges in the spatial domain}) the problem of convolution on the edges, but this time in the frequency domain. Understanding the sampling theorem and the discrete Fourier transform is very important in order to be able to pull out valuable science from the discrete image pixels. Therefore we have included the mathematical proofs and figures so you can have a clear understanding of these very important concepts. @menu * Fourier series historical background:: Historical background. * Circles and the complex plane:: Interpreting complex numbers. * Fourier series:: Fourier Series definition. * Fourier transform:: Fourier Transform definition. * Dirac delta and comb:: Dirac delta and Dirac comb. * Convolution theorem:: Derivation of Convolution theorem. * Sampling theorem:: Sampling theorem (Nyquist frequency). * Discrete Fourier transform:: Derivation and explanation of DFT. * Fourier operations in two dimensions:: Extend to 2D images. * Edges in the frequency domain:: Interpretation of edge effects. @end menu @node Fourier series historical background, Circles and the complex plane, Frequency domain and Fourier operations, Frequency domain and Fourier operations @subsubsection Fourier series historical background Ever since the ancient times, the circle has been (and still is) the simplest shape for abstract comprehension. All you need is a center point and a radius and you are done. All the points on a circle are at a fixed distance from the center. However, the moment you try to connect this elegantly simple and beautiful abstract construct (the circle) with the real world (for example compute its area or its circumference), things become really hard (ideally, impossible) because the irrational number @mymath{\pi} gets involved. The key to understanding the Fourier series (thus the Fourier transform and finally the Discrete Fourier Transform) is our ancient desire to express everything in terms of circles or the most exceptionally simple and elegant abstract human construct. Most people prefer to say the same thing in a more ahistorical manner: to break a function into sines and cosines. As the term ``ancient'' in the previous sentence implies, Jean-Baptiste Joseph Fourier (1768 -- 1830 A.D.) was not the first person to do this. The main reason we know this process by his name today is that he came up with an ingenious method to find the necessary coefficients (radius of) and frequencies (``speed'' of rotation on) the circles for any generic (integrable) function. @float Figure,epicycle @c Since these links are long, we had to write them like this so they don't @c jump out of the text width. @image{gnuastro-figures/epicycles, 15.2cm, , Middle ages epicycles along with two demonstrations of breaking a generic function using epicycles.} @caption{Epicycles and the Fourier series. Left: A demonstration of Mercury's epicycles relative to the ``center of the world'' by Qutb al-Din al-Shirazi (1236 -- 1311 A.D.) retrieved @url{https://commons.wikimedia.org/wiki/File:Ghotb2.jpg, from Wikipedia}. @url{https://commons.wikimedia.org/wiki/File:Fourier_series_square_wave_circles_animation.gif, Middle} and Right: How adding more epicycles (or terms in the Fourier series) will approximate functions. The @url{https://commons.wikimedia.org/wiki/File:Fourier_series_sawtooth_wave_circles_animation.gif, right} animation is also available.} @end float Like most aspects of mathematics, this process of interpreting everything in terms of circles, began for astronomical purposes. When astronomers noticed that the orbit of Mars and other outer planets, did not appear to be a simple circle (as everything should have been in the heavens). At some point during their orbit, the revolution of these planets would become slower, stop, go back a little (in what is known as the retrograde motion) and then continue going forward again. The correction proposed by Ptolemy (90 -- 168 A.D.) was the most agreed upon. He put the planets on Epicycles or circles whose center itself rotates on a circle whose center is the earth. Eventually, as observations became more and more precise, it was necessary to add more and more epicycles in order to explain the complex motions of the planets@footnote{See the Wikipedia page on ``Deferent and epicycle'' for a more complete historical review.}. @ref{epicycle}(Left) shows an example depiction of the epicycles of Mercury in the late 13th century. Of course we now know that if they had abdicated the Earth from its throne in the center of the heavens and allowed the Sun to take its place, everything would become much simpler and true. But there wasn't enough observational evidence for changing the ``professional consensus'' of the time to this radical view suggested by a small minority@footnote{Aristarchus of Samos (310 -- 230 B.C.) appears to be one of the first people to suggest the Sun being in the center of the universe. This approach to science (that the standard model is defined by consensus) and the fact that this consensus might be completely wrong still applies equally well to our models of particle physics and cosmology today.}. So the pre-Galilean astronomers chose to keep Earth in the center and find a correction to the models (while keeping the heavens a purely ``circular'' order). The main reason we are giving this historical background which might appear off topic is to give historical evidence that while such ``approximations'' do work and are very useful for pragmatic reasons (like measuring the calendar from the movement of astronomical bodies). They offer no physical insight. The astronomers who were involved with the Ptolemaic world view had to add a huge number of epicycles during the centuries after Ptolemy in order to explain more accurate observations. Finally the death knell of this world-view was Galileo's observations with his new instrument (the telescope). So the physical insight, which is what Astronomers and Physicists are interested in (as opposed to Mathematicians and Engineers who just like proving and optimizing or calculating!) comes from being creative and not limiting our selves to such approximations. Even when they work. @node Circles and the complex plane, Fourier series, Fourier series historical background, Frequency domain and Fourier operations @subsubsection Circles and the complex plane Before going onto the derivation, it is also useful to review how the complex numbers and their plane relate to the circles we talked about above. The two schematics in the middle and right of @ref{epicycle} show how a 1D function of time can be made using the 2D real and imaginary surface. Seeing the animation in Wikipedia will really help in understanding this important concept. At each point in time, we take the vertical coordinate of the point and use it to find the value of the function at that point in time. @ref{iandtime} shows this relation with the axes marked. Leonhard Euler@footnote{Other forms of this equation were known before Euler. For example in 1707 A.D. (the year of Euler's birth) Abraham de Moivre (1667 -- 1754 A.D.) showed that @mymath{(\cos{x}+i\sin{x})^n=\cos(nx)+i\sin(nx)}. In 1714 A.D., Roger Cotes (1682 -- 1716 A.D. a colleague of Newton who proofread the second edition of Principia) showed that: @mymath{ix=\ln(\cos{x}+i\sin{x})}.} (1707 -- 1783 A.D.) showed that the complex exponential (@mymath{e^{iv}} where @mymath{v} is real) is periodic and can be written as: @mymath{e^{iv}=\cos{v}+isin{v}}. Therefore @mymath{e^{iv+2\pi}=e^{iv}}. Later, Caspar Wessel (mathematician and cartographer 1745 -- 1818 A.D.) showed how complex numbers can be displayed as vectors on a plane. Euler's identity might seem counter intuitive at first, so we will try to explain it geometrically (for deeper physical insight). On the real-imaginary 2D plane (like the left hand plot in each box of @ref{iandtime}), multiplying a number by @mymath{i} can be interpreted as rotating the point by @mymath{90} degrees (for example the value @mymath{3} on the real axis becomes @mymath{3i} on the imaginary axis). On the other hand, @mymath{e\equiv\lim_{n\rightarrow\infty}(1+{1\over n})^n}, therefore, defining @mymath{m\equiv nu}, we get: @dispmath{e^{u}=\lim_{n\rightarrow\infty}\left(1+{1\over n}\right)^{nu} =\lim_{n\rightarrow\infty}\left(1+{u\over nu}\right)^{nu} =\lim_{m\rightarrow\infty}\left(1+{u\over m}\right)^{m}} @noindent Taking @mymath{u\equiv iv} the result can be written as a generic complex number (a function of @mymath{v}): @dispmath{e^{iv}=\lim_{m\rightarrow\infty}\left(1+i{v\over m}\right)^{m}=a(v)+ib(v)} @noindent For @mymath{v=\pi}, a nice geometric animation of going to the limit can be seen @url{https://commons.wikimedia.org/wiki/File:ExpIPi.gif, on Wikipedia}. We see that @mymath{\lim_{m\rightarrow\infty}a(\pi)=-1}, while @mymath{\lim_{m\rightarrow\infty}b(\pi)=0}, which gives the famous @mymath{e^{i\pi}=-1} equation. The final value is the real number @mymath{-1}, however the distance of the polygon points traversed as @mymath{m\rightarrow\infty} is half the circumference of a circle or @mymath{\pi}, showing how @mymath{v} in the equation above can be interpreted as an angle in units of radians and therefore how @mymath{a(v)=cos(v)} and @mymath{b(v)=sin(v)}. Since @mymath{e^{iv}} is periodic (let's assume with a period of @mymath{T}), it is more clear to write it as @mymath{v\equiv{2{\pi}n\over T}t} (where @mymath{n} is an integer), so @mymath{e^{iv}=e^{i{2{\pi}n\over T}t}}. The advantage of this notation is that the period (@mymath{T}) is clearly visible and the frequency (@mymath{2{\pi}n \over T}, in units of 1/cycle) is defined through the integer @mymath{n}. In this notation, @mymath{t} is in units of ``cycle''s. As we see from the examples in @ref{epicycle} and @ref{iandtime}, for each constituting frequency, we need a respective `magnitude' or the radius of the circle in order to accurately approximate the desired 1D function. The concepts of ``period'' and ``frequency'' are relatively easy to grasp when using temporal units like time because this is how we define them in every-day life. However, in an image (astronomical data), we are dealing with spatial units like distance. Therefore, by one ``period'' we mean the @emph{distance} at which the signal is identical and frequency is defined as the inverse of that spatial ``period''. The complex circle of @ref{iandtime} can be thought of the Moon rotating about Earth which is rotating around the Sun; so the ``Real (signal)'' axis shows the Moon's position as seen by a distant observer on the Sun as time goes by. Because of the scalar (not having any direction or vector) nature of time, @ref{iandtime} is easier to understand in units of time. When thinking about spatial units, mentally replace the ``Time (sec)'' axis with ``Distance (meters)''. Because length has direction and is a vector, visualizing the rotation of the imaginary circle and the advance along the ``Distance (meters)'' axis is not as simple as temporal units like time. @float Figure,iandtime @image{gnuastro-figures/iandtime, 15.2cm, , } @caption{Relation between the real (signal), imaginary (@mymath{i\equiv\sqrt{-1}}) and time axes at two snapshots of time.} @end float @node Fourier series, Fourier transform, Circles and the complex plane, Frequency domain and Fourier operations @subsubsection Fourier series In astronomical images, our variable (brightness, or number of photo-electrons, or signal to be more generic) is recorded over the 2D spatial surface of a camera pixel. However to make things easier to understand, here we will assume that the signal is recorded in 1D (assume one row of the 2D image pixels). Also for this section and the next (@ref{Fourier transform}) we will be talking about the signal before it is digitized or pixelated. Let's assume that we have the continuous function @mymath{f(l)} which is integrable in the interval @mymath{[l_0, l_0+L]} (always true in practical cases like images). Take @mymath{l_0} as the position of the first pixel in the assumed row of the image and @mymath{L} as the width of the image along that row. The units of @mymath{l_0} and @mymath{L} can be in any spatial units (for example meters) or an angular unit (like radians) multiplied by a fixed distance which is more common. To approximate @mymath{f(l)} over this interval, we need to find a set of frequencies and their corresponding `magnitude's (see @ref{Circles and the complex plane}). Therefore our aim is to show @mymath{f(l)} as the following sum of periodic functions: @dispmath{ f(l)=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over L}l} } @noindent Note that the different frequencies (@mymath{2{\pi}n/L}, in units of cycles per meters for example) are not arbitrary. They are all integer multiples of the fundamental frequency of @mymath{\omega_0=2\pi/L}. Recall that @mymath{L} was the length of the signal we want to model. Therefore, we see that the smallest possible frequency (or the frequency resolution) in the end, depends on the length we observed the signal or @mymath{L}. In the case of each dimension on an image, this is the size of the image in the respective dimension. The frequencies have been defined in this ``harmonic'' fashion to insure that the final sum is periodic outside of the @mymath{[l_0, l_0+L]} interval too. At this point, you might be thinking that the sky is not periodic with the same period as my camera's view angle. You are absolutely right! The important thing is that since your camera's observed region is the only region we are ``observing'' and will be using, the rest of the sky is irrelevant; so we can safely assume the sky is periodic outside of it. However, this working assumption will haunt us later in @ref{Edges in the frequency domain}. The frequencies are thus determined by definition. So all we need to do is to find the coefficients (@mymath{c_n}), or magnitudes, or radii of the circles for each frequency which is identified with the integer @mymath{n}. Fourier's approach was to multiply both sides with a fixed term: @dispmath{ f(l)e^{-i{2{\pi}m\over L}l}=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l} } @noindent where @mymath{m>0}@footnote{ We could have assumed @mymath{m<0} and set the exponential to positive, but this is more clear.}. We can then integrate both sides over the observation period: @dispmath{ \int_{l_0}^{l_0+L}f(l)e^{-i{2{\pi}m\over L}l}dl =\int_{l_0}^{l_0+L}\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}(n-m)\over L}l}dl=\displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+L}e^{i{2{\pi}(n-m)\over L}l}dl } @noindent Both @mymath{n} and @mymath{m} are positive integers. Also, we know that a complex exponential is periodic so after one period (@mymath{L}) it comes back to its starting point. Therefore @mymath{\int_{l_0}^{l_0+L}e^{2{\pi}k/L}dl=0} for any @mymath{k>0}. However, when @mymath{k=0}, this integral becomes: @mymath{\int_{l_0}^{l_0+T}e^0dt=\int_{l_0}^{l_0+T}dt=T}. Hence since the integral will be zero for all @mymath{n{\neq}m}, we get: @dispmath{ \displaystyle\sum_{n=-\infty}^{\infty}c_n\int_{l_0}^{l_0+T}e^{i{2{\pi}(n-m)\over L}l}dl=Lc_m } @noindent The origin of the axis is fundamentally an arbitrary position. So let's set it to the start of the image such that @mymath{l_0=0}. So we can find the ``magnitude'' of the frequency @mymath{2{\pi}m/L} within @mymath{f(l)} through the relation: @dispmath{ c_m={1\over L}\int_{0}^{L}f(l)e^{-i{2{\pi}m\over L}l}dl } @node Fourier transform, Dirac delta and comb, Fourier series, Frequency domain and Fourier operations @subsubsection Fourier transform In @ref{Fourier series}, we had to assume that the function is periodic outside of the desired interval with a period of @mymath{L}. Therefore, assuming that @mymath{L\rightarrow\infty} will allow us to work with any function. However, with this approximation, the fundamental frequency (@mymath{\omega_0}) or the frequency resolution that we discussed in @ref{Fourier series} will tend to zero: @mymath{\omega_0\rightarrow0}. In the equation to find @mymath{c_m}, every @mymath{m} represented a frequency (multiple of @mymath{\omega_0}) and the integration on @mymath{l} removes the dependence of the right side of the equation on @mymath{l}, making it only a function of @mymath{m} or frequency. Let's define the following two variables: @dispmath{\omega{\equiv}m\omega_0={2{\pi}m\over L}} @dispmath{F(\omega){\equiv}Lc_m} @noindent The equation to find the coefficients of each frequency in @ref{Fourier series} thus becomes: @dispmath{ F(\omega)=\int_{-\infty}^{\infty}f(l)e^{-i{\omega}l}dl. } @noindent The function @mymath{F(\omega)} is thus the @emph{Fourier transform} of @mymath{f(l)} in the frequency domain. So through this transformation, we can find (analyze) the magnitudes of the constituting frequencies or the value in the frequency space@footnote{As we discussed before, this `magnitude' can be interpreted as the radius of the circle rotating at this frequency in the epicyclic interpretation of the Fourier series, see @ref{epicycle} and @ref{iandtime}.} of our spatial input function. The great thing is that we can also do the reverse and later synthesize the input function from its Fourier transform. Let's do it: with the approximations above, multiply the right side of the definition of the Fourier Series (@ref{Fourier series}) with @mymath{1=L/L=({\omega_0}L)/(2\pi)}: @dispmath{ f(l)={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}Lc_ne^{{2{\pi}in\over L}l}\omega_0={1\over 2\pi}\displaystyle\sum_{n=-\infty}^{\infty}F(\omega)e^{i{\omega}l}\Delta\omega } @noindent To find the right most side of this equation, we renamed @mymath{\omega_0} as @mymath{\Delta\omega} because it was our resolution, @mymath{2{\pi}n/L} was written as @mymath{\omega} and finally, @mymath{Lc_n} was written as @mymath{F(\omega)} as we defined above. Now, as @mymath{L\rightarrow\infty}, @mymath{\Delta\omega\rightarrow0} so we can write: @dispmath{ f(l)={1\over 2\pi}\int_{-\infty}^{\infty}F(\omega)e^{i{\omega}l}d\omega } Together, these two equations provide us with a very powerful set of tools that we can use to process (analyze) and recreate (synthesize) the input signal. Through the first equation, we can break up our input function into its constituent frequencies and analyze it, hence it is also known as @emph{analysis}. Using the second equation, we can synthesize or make the input function from the known frequencies and their magnitudes. Thus it is known as @emph{synthesis}. Here, we symbolize the Fourier transform (analysis) and its inverse (synthesis) of a function @mymath{f(l)} and its Fourier Transform @mymath{F(\omega)} as @mymath{{\cal F}[f]} and @mymath{{\cal F}^{-1}[F]}. @node Dirac delta and comb, Convolution theorem, Fourier transform, Frequency domain and Fourier operations @subsubsection Dirac delta and comb The Dirac @mymath{\delta} (delta) function (also known as an impulse) is the way that we convert a continuous function into a discrete one. It is defined to satisfy the following integral: @dispmath{\int_{-\infty}^{\infty}\delta(l)dl=1} @noindent When integrated with another function, it gives that function's value at @mymath{l=0}: @dispmath{\int_{-\infty}^{\infty}f(l)\delta(l)dt=f(0)} @noindent An impulse positioned at another point (say @mymath{l_0}) is written as @mymath{\delta(l-l_0)}: @dispmath{\int_{-\infty}^{\infty}f(l)\delta(l-l_0)dt=f(l_0)} @noindent The Dirac @mymath{\delta} function also operates similarly if we use summations instead of integrals. The Fourier transform of the delta function is: @dispmath{{\cal F}[\delta(l)]=\int_{-\infty}^{\infty}\delta(l)e^{-i{\omega}l}dl=e^{-i{\omega}0}=1} @dispmath{{\cal F}[\delta(l-l_0)]=\int_{-\infty}^{\infty}\delta(l-l_0)e^{-i{\omega}l}dl=e^{-i{\omega}l_0}} @noindent From the definition of the Dirac @mymath{\delta} we can also define a Dirac comb (@mymath{{\rm III}_P}) or an impulse train with infinite impulses separated by @mymath{P}: @dispmath{ {\rm III}_P(l)\equiv\displaystyle\sum_{k=-\infty}^{\infty}\delta(l-kP) } @noindent @mymath{P} is chosen to represent ``pixel width'' later in @ref{Sampling theorem}. Therefore the Dirac comb is periodic with a period of @mymath{P}. We have intentionally used a different name for the period of the Dirac comb compared to the input signal's length of observation that we showed with @mymath{L} in @ref{Fourier series}. This difference is highlighted here to avoid confusion later when these two periods are needed together in @ref{Discrete Fourier transform}. The Fourier transform of the Dirac comb will be necessary in @ref{Sampling theorem}, so let's derive it. By its definition, it is periodic, with a period of @mymath{P}, so the Fourier coefficients of its Fourier Series (@ref{Fourier series}) can be calculated within one period: @dispmath{{\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}c_ne^{i{2{\pi}n\over P}l}} @noindent We can now find the @mymath{c_n} from @ref{Fourier series}: @dispmath{ c_n={1\over P}\int_{-P/2}^{P/2}\delta(l)e^{-i{2{\pi}n\over P}l} ={1\over P}\quad\quad \rightarrow \quad\quad {\rm III}_P={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}e^{i{2{\pi}n\over P}l} } @noindent So we can write the Fourier transform of the Dirac comb as: @dispmath{ {\cal F}[{\rm III}_P]=\int_{-\infty}^{\infty}{\rm III}_Pe^{-i{\omega}l}dl ={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}e^{-i(\omega-{2{\pi}n\over P})l}dl={1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\delta\left(\omega-{2{\pi}n\over P}\right) } @noindent In the last step, we used the fact that the complex exponential is a periodic function, that @mymath{n} is an integer and that as we defined in @ref{Fourier transform}, @mymath{\omega{\equiv}m\omega_0}, where @mymath{m} was an integer. The integral will be zero for any @mymath{\omega} that is not equal to @mymath{2{\pi}n/P}, a more complete explanation can be seen in @ref{Fourier series}. Therefore, while in the spatial domain the impulses had spacing of @mymath{P} (meters for example), in the frequency space, the spacing between the different impulses are @mymath{2\pi/P} cycles per meters. @node Convolution theorem, Sampling theorem, Dirac delta and comb, Frequency domain and Fourier operations @subsubsection Convolution theorem The convolution (shown with the @mymath{\ast} operator) of the two functions @mymath{f(l)} and @mymath{h(l)} is defined as: @dispmath{ c(l)\equiv[f{\ast}h](l)=\int_{-\infty}^{\infty}f(\tau)h(l-\tau)d\tau } @noindent See @ref{Convolution process} for a more detailed physical (pixel based) interpretation of this definition. The Fourier transform of convolution (@mymath{C(\omega)}) can be written as: @dispmath{ C(\omega)=\int_{-\infty}^{\infty}[f{\ast}h](l)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}f(\tau)\left[\int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl\right]d\tau } @noindent To solve the inner integral, let's define @mymath{s{\equiv}l-\tau}, so that @mymath{ds=dl} and @mymath{l=s+\tau} then the inner integral becomes: @dispmath{ \int_{-\infty}^{\infty}h(l-\tau)e^{-i{\omega}l}dl= \int_{-\infty}^{\infty}h(s)e^{-i{\omega}(s+\tau)}ds=e^{-i{\omega}\tau}\int_{-\infty}^{\infty}h(s)e^{-i{\omega}s}ds=H(\omega)e^{-i{\omega}\tau} } @noindent where @mymath{H(\omega)} is the Fourier transform of @mymath{h(l)}. Substituting this result for the inner integral above, we get: @dispmath{ C(\omega)=H(\omega)\int_{-\infty}^{\infty}f(\tau)e^{-i{\omega}\tau}d\tau=H(\omega)F(\omega)=F(\omega)H(\omega) } @noindent where @mymath{F(\omega)} is the Fourier transform of @mymath{f(l)}. So multiplying the Fourier transform of two functions individually, we get the Fourier transform of their convolution. The convolution theorem also proves a relation between the convolutions in the frequency space. Let's define: @dispmath{D(\omega){\equiv}F(\omega){\ast}H(\omega)} @noindent Applying the inverse Fourier Transform or synthesis equation (@ref{Fourier transform}) to both sides and following the same steps above, we get: @dispmath{d(l)=f(l)h(l)} @noindent Where @mymath{d(l)} is the inverse Fourier transform of @mymath{D(\omega)}. We can therefore re-write the two equations above formally as the convolution theorem: @dispmath{ {\cal F}[f{\ast}h]={\cal F}[f]{\cal F}[h] } @dispmath{ {\cal F}[fh]={\cal F}[f]\ast{\cal F}[h] } Besides its usefulness in blurring an image by convolving it with a given kernel, the convolution theorem also enables us to do another very useful operation in data analysis: to match the blur (or PSF) between two images taken with different telescopes/cameras or under different atmospheric conditions. This process is also known as de-convolution. Let's take @mymath{f(l)} as the image with a narrower PSF (less blurry) and @mymath{c(l)} as the image with a wider PSF which appears more blurred. Also let's take @mymath{h(l)} to represent the kernel that should be convolved with the sharper image to create the more blurry image. Above, we proved the relation between these three images through the convolution theorem. But there, we assumed that @mymath{f(l)} and @mymath{h(l)} are known (given) and the convolved image is desired. In de-convolution, we have @mymath{f(l)} --the sharper image-- and @mymath{f*h(l)} --the more blurry image-- and we want to find the kernel @mymath{h(l)}. The solution is a direct result of the convolution theorem: @dispmath{ {\cal F}[h]={{\cal F}[f{\ast}h]\over {\cal F}[f]} \quad\quad {\rm or} \quad\quad h(l)={\cal F}^{-1}\left[{{\cal F}[f{\ast}h]\over {\cal F}[f]}\right] } While this works really nice, it has two problems: @itemize @item If @mymath{{\cal F}[f]} has any zero values, then the inverse Fourier transform will not be a number! @item If there is significant noise in the image, then the high frequencies of the noise are going to significantly reduce the quality of the final result. @end itemize A standard solution to both these problems is the Weiner de-convolution algorithm@footnote{@url{https://en.wikipedia.org/wiki/Wiener_deconvolution}}. @node Sampling theorem, Discrete Fourier transform, Convolution theorem, Frequency domain and Fourier operations @subsubsection Sampling theorem Our mathematical functions are continuous, however, our data collecting and measuring tools are discrete. Here we want to give a mathematical formulation for digitizing the continuous mathematical functions so that later, we can retrieve the continuous function from the digitized recorded input. Assuming that we have a continuous function @mymath{f(l)}, then we can define @mymath{f_s(l)} as the `sampled' @mymath{f(l)} through the Dirac comb (see @ref{Dirac delta and comb}): @dispmath{ f_s(l)=f(l){\rm III}_P=\displaystyle\sum_{n=-\infty}^{\infty}f(l)\delta(l-nP) } @noindent The discrete data-element @mymath{f_k} (for example, a pixel in an image), where @mymath{k} is an integer, can thus be represented as: @dispmath{f_k=\int_{-\infty}^{\infty}f_s(l)dl=\int_{-\infty}^{\infty}f(l)\delta(l-kP)dt=f(kP)} Note that in practice, our discrete data points are not found in this fashion. Each detector pixel (in an image for example) has an area and averages the signal it receives over that area, not a mathematical point as the Dirac @mymath{\delta} function defines. However, as long as the variation in the signal over one detector pixel is not significant, this can be a good approximation. Having put this issue to the side, we can now try to find the relation between the Fourier transforms of the un-sampled @mymath{f(l)} and the sampled @mymath{f_s(l)}. For a more clear notation, let's define: @dispmath{F_s(\omega)\equiv{\cal F}[f_s]} @dispmath{D(\omega)\equiv{\cal F}[{\rm III}_P]} @noindent Then using the Convolution theorem (see @ref{Convolution theorem}), @mymath{F_s(\omega)} can be written as: @dispmath{F_s(\omega)={\cal F}[f(l){\rm III}_P]=F(\omega){\ast}D(\omega)} @noindent Finally, from the definition of convolution and the Fourier transform of the Dirac comb (see @ref{Dirac delta and comb}), we get: @dispmath{ \eqalign{ F_s(\omega) &= \int_{-\infty}^{\infty}F(\omega)D(\omega-\mu)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}\int_{-\infty}^{\infty}F(\omega)\delta\left(\omega-\mu-{2{\pi}n\over P}\right)d\mu \cr &= {1\over P}\displaystyle\sum_{n=-\infty}^{\infty}F\left( \omega-{2{\pi}n\over P}\right).\cr } } @mymath{F(\omega)} was only a simple function, see @ref{samplingfreq}(left). However, from the sampled Fourier transform function we see that @mymath{F_s(\omega)} is the superposition of infinite copies of @mymath{F(\omega)} that have been shifted, see @ref{samplingfreq}(right). From the equation, it is clear that the shift in each copy is @mymath{2\pi/P}. @float Figure,samplingfreq @image{gnuastro-figures/samplingfreq, 15.2cm, , } @caption{Sampling causes infinite repetition in the frequency domain. FT is an abbreviation for `Fourier transform'. @mymath{\omega_m} represents the maximum frequency present in the input. @mymath{F(\omega)} is only symmetric on both sides of 0 when the input is real (not complex). In general @mymath{F(\omega)} is complex and thus cannot be simply plotted like this. Here we have assumed a real Gaussian @mymath{f(t)} which has produced a Gaussian @mymath{F(\omega)}.} @end float The input @mymath{f(l)} can have any distribution of frequencies in it. In the example of @ref{samplingfreq}(left), the input consisted of a range of frequencies equal to @mymath{\Delta\omega=2\omega_m}. Fortunately as @ref{samplingfreq}(right) shows, the assumed pixel size (@mymath{P}) we used to sample this hypothetical function was such that @mymath{2\pi/P>\Delta\omega}. The consequence is that each copy of @mymath{F(\omega)} has become completely separate from the surrounding copies. Such a digitized (sampled) data set is thus called @emph{over-sampled}. When @mymath{2\pi/P=\Delta\omega}, @mymath{P} is just small enough to finely separate even the largest frequencies in the input signal and thus it is known as @emph{critically-sampled}. Finally if @mymath{2\pi/P<\Delta\omega} we are dealing with an @emph{under-sampled} data set. In an under-sampled data set, the separate copies of @mymath{F(\omega)} are going to overlap and this will deprive us of recovering high constituent frequencies of @mymath{f(l)}. The effects of under-sampling in an image with high rates of change (for example a brick wall imaged from a distance) can clearly be visually seen and is known as @emph{aliasing}. When the input @mymath{f(l)} is composed of a finite range of frequencies, @mymath{f(l)} is known as a @emph{band-limited} function. The example in @ref{samplingfreq}(left) was a nice demonstration of such a case: for all @mymath{\omega<-\omega_m} or @mymath{\omega>\omega_m}, we have @mymath{F(\omega)=0}. Therefore, when the input function is band-limited and our detector's pixels are placed such that we have critically (or over-) sampled it, then we can exactly reproduce the continuous @mymath{f(l)} from the discrete or digitized samples. To do that, we just have to isolate one copy of @mymath{F(\omega)} from the infinite copies and take its inverse Fourier transform. This ability to exactly reproduce the continuous input from the sampled or digitized data leads us to the @emph{sampling theorem} which connects the inherent property of the continuous signal (its maximum frequency) to that of the detector (the spacing between its pixels). The sampling theorem states that the full (continuous) signal can be recovered when the pixel size (@mymath{P}) and the maximum constituent frequency in the signal (@mymath{\omega_m}) have the following relation@footnote{This equation is also shown in some places without the @mymath{2\pi}. Whether @mymath{2\pi} is included or not depends on how you define the frequency}: @dispmath{{2\pi\over P}>2\omega_m} @noindent This relation was first formulated by Harry Nyquist (1889 -- 1976 A.D.) in 1928 and formally proved in 1949 by Claude E. Shannon (1916 -- 2001 A.D.) in what is now known as the Nyquist-Shannon sampling theorem. In signal processing, the signal is produced (synthesized) by a transmitter and is received and de-coded (analyzed) by a receiver. Therefore producing a band-limited signal is necessary. In astronomy, we do not produce the shapes of our targets, we are only observers. Galaxies can have any shape and size, therefore ideally, our signal is not band-limited. However, since we are always confined to observing through an aperture, the aperture will cause a point source (for which @mymath{\omega_m=\infty}) to be spread over several pixels. This spread is quantitatively known as the point spread function or PSF. This spread does blur the image which is undesirable; however, for this analysis it produces the positive outcome that there will be a finite @mymath{\omega_m}. Though we should caution that any detector will have noise which will add lots of very high frequency (ideally infinite) changes between the pixels. However, the coefficients of those noise frequencies are usually exceedingly small. @node Discrete Fourier transform, Fourier operations in two dimensions, Sampling theorem, Frequency domain and Fourier operations @subsubsection Discrete Fourier transform As we have stated several times so far, the input image is a digitized, pixelated or discrete array of values (@mymath{f_s(l)}, see @ref{Sampling theorem}). The input is not a continuous function. Also, all our numerical calculations can only be done on a sampled, or discrete Fourier transform. Note that @mymath{F_s(\omega)} is not discrete, it is continuous. One way would be to find the analytic @mymath{F_s(\omega)}, then sample it at any desired ``freq-pixel''@footnote{We are using the made-up word ``freq-pixel'' so they are not confused with spatial domain ``pixels''.} spacing. However, this process would involve two steps of operations and computers in particular are not too good at analytic operations for the first step. So here, we will derive a method to directly find the `freq-pixel'ated @mymath{F_s(\omega)} from the pixelated @mymath{f_s(l)}. Let's start with the definition of the Fourier transform (see @ref{Fourier transform}): @dispmath{F_s(\omega)=\int_{-\infty}^{\infty}f_s(l)e^{-i{\omega}l}dl } @noindent From the definition of @mymath{f_s(\omega)} (using @mymath{x} instead of @mymath{n}) we get: @dispmath{ \eqalign{ F_s(\omega) &= \displaystyle\sum_{x=-\infty}^{\infty} \int_{-\infty}^{\infty}f(l)\delta(l-xP)e^{-i{\omega}l}dl \cr &= \displaystyle\sum_{x=-\infty}^{\infty} f_xe^{-i{\omega}xP} } } @noindent Where @mymath{f_x} is the value of @mymath{f(l)} on the point @mymath{x} or the value of the @mymath{x}th pixel. As shown in @ref{Sampling theorem} this function is infinitely periodic with a period of @mymath{2\pi/P}. So all we need is the values within one period: @mymath{0<\omega<2\pi/P}, see @ref{samplingfreq}. We want @mymath{X} samples within this interval, so the frequency difference between each frequency sample or freq-pixel is @mymath{1/XP}. Hence we will evaluate the equation above on the points at: @dispmath{\omega={u\over XP} \quad\quad u = 0, 1, 2, ..., X-1} @noindent Therefore the value of the freq-pixel @mymath{u} in the frequency domain is: @dispmath{F_u=\displaystyle\sum_{x=0}^{X-1} f_xe^{-i{ux\over X}} } @noindent Therefore, we see that for each freq-pixel in the frequency domain, we are going to need all the pixels in the spatial domain@footnote{So even if one pixel is a blank pixel (see @ref{Blank pixels}), all the pixels in the frequency domain will also be blank.}. If the input (spatial) pixel row is also @mymath{X} pixels wide, then we can exactly recover the @mymath{x}th pixel with the following summation: @dispmath{f_x={1\over X}\displaystyle\sum_{u=0}^{X-1} F_ue^{i{ux\over X}} } When the input pixel row (we are still only working on 1D data) has @mymath{X} pixels, then it is @mymath{L=XP} spatial units wide. @mymath{L}, or the length of the input data was defined in @ref{Fourier series} and @mymath{P} or the space between the pixels in the input was defined in @ref{Dirac delta and comb}. As we saw in @ref{Sampling theorem}, the input (spatial) pixel spacing (@mymath{P}) specifies the range of frequencies that can be studied and in @ref{Fourier series} we saw that the length of the (spatial) input, (@mymath{L}) determines the resolution (or size of the freq-pixels) in our discrete Fourier transformed image. Both result from the fact that the frequency domain is the inverse of the spatial domain. @node Fourier operations in two dimensions, Edges in the frequency domain, Discrete Fourier transform, Frequency domain and Fourier operations @subsubsection Fourier operations in two dimensions Once all the relations in the previous sections have been clearly understood in one dimension, it is very easy to generalize them to two or even more dimensions since each dimension is by definition independent. Previously we defined @mymath{l} as the continuous variable in 1D and the inverse of the period in its direction to be @mymath{\omega}. Let's show the second spatial direction with @mymath{m} the the inverse of the period in the second dimension with @mymath{\nu}. The Fourier transform in 2D (see @ref{Fourier transform}) can be written as: @dispmath{F(\omega, \nu)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} f(l, m)e^{-i({\omega}l+{\nu}m)}dl} @dispmath{f(l, m)=\int_{-\infty}^{\infty}\int_{-\infty}^{\infty} F(\omega, \nu)e^{i({\omega}l+{\nu}m)}dl} The 2D Dirac @mymath{\delta(l,m)} is non-zero only when @mymath{l=m=0}. The 2D Dirac comb (or Dirac brush! See @ref{Dirac delta and comb}) can be written in units of the 2D Dirac @mymath{\delta}. For most image detectors, the sides of a pixel are equal in both dimensions. So @mymath{P} remains unchanged, if a specific device is used which has non-square pixels, then for each dimension a different value should be used. @dispmath{{\rm III}_P(l, m)\equiv\displaystyle\sum_{j=-\infty}^{\infty} \displaystyle\sum_{k=-\infty}^{\infty} \delta(l-jP, m-kP) } The Two dimensional Sampling theorem (see @ref{Sampling theorem}) is thus very easily derived as before since the frequencies in each dimension are independent. Let's take @mymath{\nu_m} as the maximum frequency along the second dimension. Therefore the two dimensional sampling theorem says that a 2D band-limited function can be recovered when the following conditions hold@footnote{If the pixels are not a square, then each dimension has to use the respective pixel size, but since most detectors have square pixels, we assume so here too}: @dispmath{ {2\pi\over P} > 2\omega_m \quad\quad\quad {\rm and} \quad\quad\quad {2\pi\over P} > 2\nu_m} Finally, let's represent the pixel counter on the second dimension in the spatial and frequency domains with @mymath{y} and @mymath{v} respectively. Also let's assume that the input image has @mymath{Y} pixels on the second dimension. Then the two dimensional discrete Fourier transform and its inverse (see @ref{Discrete Fourier transform}) can be written as: @dispmath{F_{u,v}=\displaystyle\sum_{x=0}^{X-1}\displaystyle\sum_{y=0}^{Y-1} f_{x,y}e^{-i({ux\over X}+{vy\over Y})} } @dispmath{f_{x,y}={1\over XY}\displaystyle\sum_{u=0}^{X-1}\displaystyle\sum_{v=0}^{Y-1} F_{u,v}e^{i({ux\over X}+{vy\over Y})} } @node Edges in the frequency domain, , Fourier operations in two dimensions, Frequency domain and Fourier operations @subsubsection Edges in the frequency domain With a good grasp of the frequency domain, we can revisit the problem of convolution on the image edges, see @ref{Edges in the spatial domain}. When we apply the convolution theorem (see @ref{Convolution theorem}) to convolve an image, we first take the discrete Fourier transforms (DFT, @ref{Discrete Fourier transform}) of both the input image and the kernel, then we multiply them with each other and then take the inverse DFT to construct the convolved image. Of course, in order to multiply them with each other in the frequency domain, the two images have to be the same size, so let's assume that we pad the kernel (it is usually smaller than the input image) with zero valued pixels in both dimensions so it becomes the same size as the input image before the DFT. Having multiplied the two DFTs, we now apply the inverse DFT which is where the problem is usually created. If the DFT of the kernel only had values of 1 (unrealistic condition!) then there would be no problem and the inverse DFT of the multiplication would be identical with the input. However in real situations, the kernel's DFT has a maximum of 1 (because the sum of the kernel has to be one, see @ref{Convolution process}) and decreases something like the hypothetical profile of @ref{samplingfreq}. So when multiplied with the input image's DFT, the coefficients or magnitudes (see @ref{Circles and the complex plane}) of the smallest frequency (or the sum of the input image pixels) remains unchanged, while the magnitudes of the higher frequencies are significantly reduced. As we saw in @ref{Sampling theorem}, the Fourier transform of a discrete input will be infinitely repeated. In the final inverse DFT step, the input is in the frequency domain (the multiplied DFT of the input image and the kernel DFT). So the result (our output convolved image) will be infinitely repeated in the spatial domain. In order to accurately reconstruct the input image, we need all the frequencies with the correct magnitudes. However, when the magnitudes of higher frequencies are decreased, longer periods (shorter frequencies) will dominate in the reconstructed pixel values. Therefore, when constructing a pixel on the edge of the image, the newly empowered longer periods will look beyond the input image edges and will find the repeated input image there. So if you convolve an image in this fashion using the convolution theorem, when a bright object exists on one edge of the image, its blurred wings will be present on the other side of the convolved image. This is often termed as circular convolution or cyclic convolution. So, as long as we are dealing with convolution in the frequency domain, there is nothing we can do about the image edges. The least we can do is to eliminate the ghosts of the other side of the image. So, we add zero valued pixels to both the input image and the kernel in both dimensions so the image that will be convolved has a size equal to the sum of both images in each dimension. Of course, the effect of this zero-padding is that the sides of the output convolved image will become dark. To put it another way, the edges are going to drain the flux from nearby objects. But at least it is consistent across all the edges of the image and is predictable. In Convolve, you can see the padded images when inspecting the frequency domain convolution steps with the @option{--viewfreqsteps} option. @node Spatial vs. Frequency domain, Convolution kernel, Frequency domain and Fourier operations, Convolve @subsection Spatial vs. Frequency domain With the discussions above it might not be clear when to choose the spatial domain and when to choose the frequency domain. Here we will try to list the benefits of each. @noindent The spatial domain, @itemize @item Can correct for the edge effects of convolution, see @ref{Edges in the spatial domain}. @item Can operate on blank pixels. @item Can be faster than frequency domain when the kernel is small (in terms of the number of pixels on the sides). @end itemize @noindent The frequency domain, @itemize @item Will be much faster when the image and kernel are both large. @end itemize @noindent As a general rule of thumb, when working on an image of modeled profiles use the frequency domain and when working on an image of real (observed) objects use the spatial domain (corrected for the edges). The reason is that if you apply a frequency domain convolution to a real image, you are going to loose information on the edges and generally you don't want large kernels. But when you have made the profiles in the image yourself, you can just make a larger input image and crop the central parts to completely remove the edge effect, see @ref{If convolving afterwards}. Also due to oversampling, both the kernels and the images can become very large and the speed boost of frequency domain convolution will significantly improve the processing time, see @ref{Oversampling}. @node Convolution kernel, Invoking astconvolve, Spatial vs. Frequency domain, Convolve @subsection Convolution kernel All the programs that need convolution will need to be given a convolution kernel file and extension. In most cases (other than Convolve, see @ref{Convolve}) the kernel file name is optional. However, the extension is necessary and must be specified either on the command-line or at least one of the configuration files (see @ref{Configuration files}). Within Gnuastro, there are two ways to create a kernel image: @itemize @item MakeProfiles: You can use MakeProfiles to create a parametric (based on a radial function) kernel, see @ref{MakeProfiles}. By default MakeProfiles will make the Gaussian and Moffat profiles in a separate file so you can feed it into any of the programs. @item ConvertType: You can write your own desired kernel into a text file table and convert it to a FITS file with ConvertType, see @ref{ConvertType}. Just be careful that the kernel has to have an odd number of pixels along its two axes, see @ref{Convolution process}. All the programs that do convolution will normalize the kernel internally, so if you choose this option, you don't have to worry about normalizing the kernel. Only within Convolve, there is an option to disable normalization, see @ref{Invoking astconvolve}. @end itemize @noindent The two options to specify a kernel file name and its extension are shown below. These are common between all the programs that will do convolution. @table @option @item -k STR @itemx --kernel=STR The convolution kernel file name. The @code{BITPIX} (data type) value of this file can be any standard type and it does not necessarily have to be normalized. Several operations will be done on the kernel image prior to the program's processing: @itemize @item It will be converted to floating point type. @item All blank pixels (see @ref{Blank pixels}) will be set to zero. @item It will be normalized so the sum of its pixels equal unity. @item It will be flipped so the convolved image has the same orientation. This is only relevant if the kernel is not circular. See @ref{Convolution process}. @end itemize @item -U STR @itemx --khdu=STR The convolution kernel HDU. Although the kernel file name is optional, before running any of the programs, they need to have a value for @option{--khdu} even if the default kernel is to be used. So be sure to keep its value in at least one of the configuration files (see @ref{Configuration files}). By default, the system configuration file has a value. @end table @node Invoking astconvolve, , Convolution kernel, Convolve @subsection Invoking Convolve Convolve an input image with a known kernel or make the kernel necessary to match two PSFs. The general template for Convolve is: @example $ astconvolve [OPTION...] ASTRdata @end example @noindent One line examples: @example ## Convolve mockimg.fits with psf.fits: $ astconvolve --kernel=psf.fits mockimg.fits ## Convolve in the spatial domain: $ astconvolve observedimg.fits --kernel=psf.fits --domain=spatial ## Find the kernel to match sharper and blurry PSF images: $ astconvolve --kernel=sharperimage.fits --makekernel=10 \ blurryimage.fits @end example The only argument accepted by Convolve is an input image file. Some of the options are the same between Convolve and some other Gnuastro programs. Therefore, to avoid repetition, they will not be repeated here. For the full list of options shared by all Gnuastro programs, please see @ref{Common options}. In particular, in the spatial domain convolve uses Gnuastro's tessellation, see @ref{Tessellation} and the common options related to that in @ref{Processing options}. Here we will only explain the options particular to Convolve. Run Convolve with @option{--help} in order to see the full list of options Convolve accepts, irrespective of where they are explained in this book. @table @option @item --nokernelflip Do not flip the kernel after reading it the spatial domain convolution. This can be useful if the flipping has already been applied to the kernel. @item --nokernelnorm Do not normalize the kernel after reading it, such that the sum of its pixels is unity. @item -d STR @itemx --domain=STR @cindex Discrete Fourier transform The domain to use for the convolution. The acceptable values are `@code{spatial}' and `@code{frequency}', corresponding to the respective domain. For large images, the frequency domain process will be more efficient than convolving in the spatial domain. However, the edges of the image will loose some flux (see @ref{Edges in the spatial domain}) and the image must not contain any blank pixels, see @ref{Spatial vs. Frequency domain}. @item --checkfreqsteps With this option a file with the initial name of the output file will be created that is suffixed with @file{_freqsteps.fits}, all the steps done to arrive at the final convolved image are saved as extensions in this file. The extensions in order are: @enumerate @item The padded input image. In frequency domain convolution the two images (input and convolved) have to be the same size and both should be padded by zeros. @item The padded kernel, similar to the above. @item @cindex Phase angle @cindex Complex numbers @cindex Numbers, complex @cindex Fourier spectrum @cindex Spectrum, Fourier The Fourier spectrum of the forward Fourier transform of the input image. Note that the Fourier transform is a complex operation (and not view able in one image!) So we either have to show the `Fourier spectrum' or the `Phase angle'. For the complex number @mymath{a+ib}, the Fourier spectrum is defined as @mymath{\sqrt{a^2+b^2}} while the phase angle is defined as @mymath{\arctan(b/a)}. @item The Fourier spectrum of the forward Fourier transform of the kernel image. @item The Fourier spectrum of the multiplied (through complex arithmetic) transformed images. @item @cindex Round-off error @cindex Floating point round-off error @cindex Error, floating point round-off The inverse Fourier transform of the multiplied image. If you open it, you will see that the convolved image is now in the center, not on one side of the image as it started with (in the padded image of the first extension). If you are working on a mock image which originally had pixels of precisely 0.0, you will notice that in those parts that your convolved profile(s) did not convert, the values are now @mymath{\sim10^{-18}}, this is due to floating-point round off errors. Therefore in the final step (when cropping the central parts of the image), we also remove any pixel with a value less than @mymath{10^{-17}}. @end enumerate @item --noedgecorrection Do not correct the edge effect in spatial domain convolution. For a full discussion, please see @ref{Edges in the spatial domain}. @item -m INT @itemx --makekernel=INT (@option{=INT}) If this option is called, Convolve will do de-convolution (see @ref{Convolution theorem}). The image specified by the @option{--kernel} option is assumed to be the sharper (less blurry) image and the input image is assumed to be the more blurry image. The value given to this option will be used as the maximum radius of the kernel. Any pixel in the final kernel that is larger than this distance from the center will be set to zero. The two images must have the same size. Noise has large frequencies which can make the result less reliable for the higher frequencies of the final result. So all the frequencies which have a spectrum smaller than the value given to the @option{minsharpspec} option in the sharper input image are set to zero and not divided. This will cause the wings of the final kernel to be flatter than they would ideally be which will make the convolved image result unreliable if it is too high. Some notes to take into account for a good result: @itemize @item Choose a bright (unsaturated) star and use a region box (with Crop for example, see @ref{Crop}) that is sufficiently above the noise. @item Use Warp (see @ref{Warp}) to warp the pixel grid so the star's center is exactly on the center of the central pixel in the cropped image. This will certainly slightly degrade the result, however, it is necessary. If there are multiple good stars, you can shift all of them, then normalize them (so the sum of each star's pixels is one) and then take their average to decrease this effect. @item The shifting might move the center of the star by one pixel in any direction, so crop the central pixel of the warped image to have a clean image for the de-convolution. @end itemize @item -c @itemx --minsharpspec (@option{=FLT}) The minimum frequency spectrum (or coefficient, or pixel value in the frequency domain image) to use in deconvolution, see the explanations under the @option{--makekernel} option for more information. @end table @node Warp, , Convolve, Data manipulation @section Warp Image warping is the process of mapping the pixels of one image onto a new pixel grid. This process is sometimes known as transformation, however following the discussion of Heckbert 1989@footnote{Paul S. Heckbert. 1989. @emph{Fundamentals of Texture mapping and Image Warping}, Master's thesis at University of California, Berkeley.} we will not be using that term because it can be confused with only pixel value or flux transformations. Here we specifically mean the pixel grid transformation which is better conveyed with `warp'. @cindex Gravitational lensing Image wrapping is a very important step in astronomy, both in observational data analysis and in simulating modeled images. In modeling, warping an image is necessary when we want to apply grid transformations to the initial models, for example in simulating gravitational lensing (Radial warpings are not yet included in Warp). Observational reasons for warping an image are listed below: @itemize @cindex Signal to noise ratio @item @strong{Noise:} Most scientifically interesting targets are inherently faint (have a very low Signal to noise ratio). Therefore one short exposure is not enough to detect such objects that are drowned deeply in the noise. We need multiple exposures so we can add them together and increase the objects' signal to noise ratio. Keeping the telescope fixed on one field of the sky is practically impossible. Therefore very deep observations have to put into the same grid before adding them. @cindex Mosaicing @cindex Image mosaic @item @strong{Resolution:} If we have multiple images of one patch of the sky (hopefully at multiple orientations) we can warp them to the same grid. The multiple orientations will allow us to `guess' the values of pixels on an output pixel grid that has smaller pixel sizes and thus increase the resolution of the output. This process of merging multiple observations is known as Mosaicing. @cindex Cosmic rays @item @strong{Cosmic rays:} Cosmic rays can randomly fall on any part of an image. If they collide vertically with the camera, they are going to create a very sharp and bright spot that in most cases can be separated easily@footnote{All astronomical targets are blurred with the PSF, see @ref{PSF}, however a cosmic ray is not and so it is very sharp (it suddenly stops at one pixel).}. However, depending on the depth of the camera pixels, and the angle that a cosmic rays collides with it, it can cover a line-like larger area on the CCD which makes the detection using their sharp edges very hard and error prone. One of the best methods to remove cosmic rays is to compare multiple images of the same field. To do that, we need all the images to be on the same pixel grid. @cindex Optical distortion @cindex Distortion, optical @item @strong{Optical distortion:} (Not yet included in Warp) In wide field images, the optical distortion that occurs on the outer parts of the focal plane will make accurate comparison of the objects at various locations impossible. It is therefore necessary to warp the image and correct for those distortions prior to the analysis. @cindex ACS @cindex CCD @cindex WFC3 @cindex Wide Field Camera 3 @cindex Charge-coupled device @cindex Hubble Space Telescope @cindex Advanced camera for surveys @item @strong{Detector not on focal plane:} In some cases (like the Hubble Space Telescope ACS and WFC3 cameras), the CCD might be tilted compared to the focal plane, therefore the recorded CCD pixels have to be projected onto the focal plane before further analysis. @end itemize @menu * Warping basics:: Basics of coordinate transformation. * Merging multiple warpings:: How to merge multiple matrices. * Resampling:: Warping an image is re-sampling it. * Invoking astwarp:: Arguments and options for Warp. @end menu @node Warping basics, Merging multiple warpings, Warp, Warp @subsection Warping basics @cindex Scaling @cindex Coordinate transformation Let's take @mymath{\left[\matrix{u&v}\right]} as the coordinates of a point in the input image and @mymath{\left[\matrix{x&y}\right]} as the coordinates of that same point in the output image@footnote{These can be any real number, we are not necessarily talking about integer pixels here.}. The simplest form of coordinate transformation (or warping) is the scaling of the coordinates, let's assume we want to scale the first axis by @mymath{M} and the second by @mymath{N}, the output coordinates of that point can be calculated by @dispmath{\left[\matrix{x\cr y}\right]= \left[\matrix{Mu\cr Nv}\right]= \left[\matrix{M&0\cr0&N}\right]\left[\matrix{u\cr v}\right]} @cindex Matrix @cindex Multiplication, Matrix @cindex Rotation of coordinates @noindent Note that these are matrix multiplications. We thus see that we can represent any such grid warping as a matrix. Another thing we can do with this @mymath{2\times2} matrix is to rotate the output coordinate around the common center of both coordinates. If the output is rotated anticlockwise by @mymath{\theta} degrees from the positive (to the right) horizontal axis, then the warping matrix should become: @dispmath{\left[\matrix{x\cr y}\right]= \left[\matrix{ucos\theta-vsin\theta\cr usin\theta+vcos\theta}\right]= \left[\matrix{cos\theta&-sin\theta\cr sin\theta&cos\theta}\right] \left[\matrix{u\cr v}\right] } @cindex Flip coordinates @noindent We can also flip the coordinates around the first axis, the second axis and the coordinate center with the following three matrices respectively: @dispmath{\left[\matrix{1&0\cr0&-1}\right]\quad\quad \left[\matrix{-1&0\cr0&1}\right]\quad\quad \left[\matrix{-1&0\cr0&-1}\right]} @cindex Shear @noindent The final thing we can do with this definition of a @mymath{2\times2} warping matrix is shear. If we want the output to be sheared along the first axis with @mymath{A} and along the second with @mymath{B}, then we can use the matrix: @dispmath{\left[\matrix{1&A\cr B&1}\right]} @noindent To have one matrix representing any combination of these steps, you use matrix multiplication, see @ref{Merging multiple warpings}. So any combinations of these transformations can be displayed with one @mymath{2\times2} matrix: @dispmath{\left[\matrix{a&b\cr c&d}\right]} @cindex Wide Field Camera 3 @cindex Hubble Space Telescope @cindex Advanced Camera for Surveys The transformations above can cover a lot of the needs of most coordinate transformations. However they are limited to mapping the point @mymath{[\matrix{0&0}]} to @mymath{[\matrix{0&0}]}. Therefore they are useless if you want one coordinate to be shifted compared to the other one. They are also space invariant, meaning that all the coordinates in the image will receive the same transformation. In other words, all the pixels in the output image will have the same area if placed over the input image. So transformations which require varying output pixel sizes like projections cannot be applied through this @mymath{2\times2} matrix either (for example for the tilted ACS and WFC3 camera detectors on board the Hubble space telescope). @cindex M@"obius, August. F. @cindex Homogeneous coordinates @cindex Coordinates, homogeneous To add these further capabilities, namely translation and projection, we use the homogeneous coordinates. They were defined about 200 years ago by August Ferdinand M@"obius (1790 -- 1868). For simplicity, we will only discuss points on a 2D plane and avoid the complexities of higher dimensions. We cannot provide a deep mathematical introduction here, interested readers can get a more detailed explanation from Wikipedia@footnote{@url{http://en.wikipedia.org/wiki/Homogeneous_coordinates}} and the references therein. By adding an extra coordinate to a point we can add the flexibility we need. The point @mymath{[\matrix{x&y}]} can be represented as @mymath{[\matrix{xZ&yZ&Z}]} in homogeneous coordinates. Therefore multiplying all the coordinates of a point in the homogeneous coordinates with a constant will give the same point. Put another way, the point @mymath{[\matrix{x&y&Z}]} corresponds to the point @mymath{[\matrix{x/Z&y/Z}]} on the constant @mymath{Z} plane. Setting @mymath{Z=1}, we get the input image plane, so @mymath{[\matrix{u&v&1}]} corresponds to @mymath{[\matrix{u&v}]}. With this definition, the transformations above can be generally written as: @dispmath{\left[\matrix{x\cr y\cr 1}\right]= \left[\matrix{a&b&0\cr c&d&0\cr 0&0&1}\right] \left[\matrix{u\cr v\cr 1}\right]} @noindent @cindex Affine Transformation @cindex Transformation, affine We thus acquired 4 extra degrees of freedom. By giving non-zero values to the zero valued elements of the last column we can have translation (try the matrix multiplication!). In general, any coordinate transformation that is represented by the matrix below is known as an affine transformation@footnote{@url{http://en.wikipedia.org/wiki/Affine_transformation}}: @dispmath{\left[\matrix{a&b&c\cr d&e&f\cr 0&0&1}\right]} @cindex Homography @cindex Projective transformation @cindex Transformation, projective We can now consider translation, but the affine transform is still spatially invariant. Giving non-zero values to the other two elements in the matrix above gives us the projective transformation or Homography@footnote{@url{http://en.wikipedia.org/wiki/Homography}} which is the most general type of transformation with the @mymath{3\times3} matrix: @dispmath{\left[\matrix{x'\cr y'\cr w}\right]= \left[\matrix{a&b&c\cr d&e&f\cr g&h&1}\right] \left[\matrix{u\cr v\cr 1}\right]} @noindent So the output coordinates can be calculated from: @dispmath{x={x' \over w}={au+bv+c \over gu+hv+1}\quad\quad\quad\quad y={y' \over w}={du+ev+f \over gu+hv+1}} Thus with Homography we can change the sizes of the output pixels on the input plane, giving a `perspective'-like visual impression. This can be quantitatively seen in the two equations above. When @mymath{g=h=0}, the denominator is independent of @mymath{u} or @mymath{v} and thus we have spatial invariance. Homography preserves lines at all orientations. A very useful fact about Homography is that its inverse is also a Homography. These two properties play a very important role in the implementation of this transformation. A short but instructive and illustrated review of affine, projective and also bi-linear mappings is provided in Heckbert 1989@footnote{Paul S. Heckbert. 1989. @emph{Fundamentals of Texture mapping and Image Warping}, Master's thesis at University of California, Berkeley. Note that since points are defined as row vectors there, the matrix is the transpose of the one discussed here.}. @node Merging multiple warpings, Resampling, Warping basics, Warp @subsection Merging multiple warpings @cindex Commutative property @cindex Matrix multiplication @cindex Multiplication, matrix @cindex Non-commutative operations @cindex Operations, non-commutative In @ref{Warping basics} we saw how a basic warp/transformation can be represented with a matrix. To make more complex warpings (for example to define a translation, rotation and scale as one warp) the individual matrices have to be multiplied through matrix multiplication. However matrix multiplication is not commutative, so the order of the set of matrices you use for the multiplication is going to be very important. The first warping should be placed as the left-most matrix. The second warping to the right of that and so on. The second transformation is going to occur on the warped coordinates of the first. As an example for merging a few transforms into one matrix, the multiplication below represents the rotation of an image about a point @mymath{[\matrix{U&V}]} anticlockwise from the horizontal axis by an angle of @mymath{\theta}. To do this, first we take the origin to @mymath{[\matrix{U&V}]} through translation. Then we rotate the image, then we translate it back to where it was initially. These three operations can be merged in one operation by calculating the matrix multiplication below: @dispmath{\left[\matrix{1&0&U\cr0&1&V\cr{}0&0&1}\right] \left[\matrix{cos\theta&-sin\theta&0\cr sin\theta&cos\theta&0\cr 0&0&1}\right] \left[\matrix{1&0&-U\cr0&1&-V\cr{}0&0&1}\right]} @node Resampling, Invoking astwarp, Merging multiple warpings, Warp @subsection Resampling @cindex Pixel @cindex Camera @cindex Detector @cindex Sampling @cindex Resampling @cindex Pixel mixing @cindex Photoelectrons @cindex Picture element @cindex Mixing pixel values A digital image is composed of discrete `picture elements' or `pixels'. When a real image is created from a camera or detector, each pixel's area is used to store the number of photo-electrons that were created when incident photons collided with that pixel's surface area. This process is called the `sampling' of a continuous or analog data into digital data. When we change the pixel grid of an image or warp it as we defined in @ref{Warping basics}, we have to `guess' the flux value of each pixel on the new grid based on the old grid, or re-sample it. Because of the `guessing', any form of warping on the data is going to degrade the image and mix the original pixel values with each other. So if an analysis can be done on an un-warped data image, it is best to leave the image untouched and pursue the analysis. However as discussed in @ref{Warp} this is not possible most of the times, so we have to accept the problem and re-sample the image. @cindex Point pixels @cindex Interpolation @cindex Bicubic interpolation @cindex Signal to noise ratio @cindex Bi-linear interpolation @cindex Interpolation, bicubic @cindex Interpolation, bi-linear In most applications of image processing, it is sufficient to consider each pixel to be a point and not an area. This assumption can significantly speed up the processing of an image and also the simplicity of the code. It is a fine assumption when the signal to noise ratio of the objects are very large. The question will then be one of interpolation because you have multiple points distributed over the output image and you want to find the values at the pixel centers. To increase the accuracy, you might also sample more than one point from within a pixel giving you more points for a more accurate interpolation in the output grid. @cindex Image edges @cindex Edges, image However, interpolation has several problems. The first one is that it will depend on the type of function you want to assume for the interpolation. For example you can choose a bi-linear or bi-cubic (the `bi's are for the 2 dimensional nature of the data) interpolation method. For the latter there are various ways to set the constants@footnote{see @url{http://entropymine.com/imageworsener/bicubic/} for a nice introduction.}. Such functional interpolation functions can fail seriously on the edges of an image. They will also need normalization so that the flux of the objects before and after the warpings are comparable. The most basic problem with such techniques is that they are based on a point while a detector pixel is an area. They add a level of subjectivity to the data (make more assumptions through the functions than the data can handle). For most applications this is fine, but in scientific applications where detection of the faintest possible galaxies or fainter parts of bright galaxies is our aim, we cannot afford this loss. Because of these reasons Warp will not use such interpolation techniques. @cindex Drizzle @cindex Pixel mixing @cindex Exact area resampling Warp will do interpolation based on ``pixel mixing''@footnote{For a graphic demonstration see @url{http://entropymine.com/imageworsener/pixelmixing/}.} or ``area resampling''. This is also what the Hubble Space Telescope pipeline calls ``Drizzling''@footnote{@url{http://en.wikipedia.org/wiki/Drizzle_(image_processing)}}. This technique requires no functions, it is thus non-parametric. It is also the closest we can get (make least assumptions) to what actually happens on the detector pixels. The basic idea is that you reverse-transform each output pixel to find which pixels of the input image it covers and what fraction of the area of the input pixels are covered. To find the output pixel value, you simply sum the value of each input pixel weighted by the overlap fraction (between 0 to 1) of the output pixel and that input pixel. Through this process, pixels are treated as an area not as a point (which is how detectors create the image), also the brightness (see @ref{Flux Brightness and magnitude}) of an object will be left completely unchanged. If there are very high spatial-frequency signals in the image (for example fringes) which vary on a scale smaller than your output image pixel size, pixel mixing can cause ailiasing@footnote{@url{http://en.wikipedia.org/wiki/Aliasing}}. So if the input image has fringes, they have to be calculated and removed separately (which would naturally be done in any astronomical application). Because of the PSF no astronomical target has a sharp change in the signal so this issue is less important for astronomical applications, see @ref{PSF}. @node Invoking astwarp, , Resampling, Warp @subsection Invoking Warp Warp an input dataset into a new grid. Any homographic warp (for example scaling, rotation, translation, projection) is acceptable, see @ref{Warping basics} for the definitions. The general template for invoking Warp is: @example $ astwarp [OPTIONS...] InputImage @end example @noindent One line examples: @example ## Rotate and then scale input image: $ astwarp --rotate=37.92 --scale=0.8 image.fits ## Scale, then translate the input image: $ astwarp --scale 8/3 --translate 2.1 image.fits ## Align raw image with celestial coordinates: $ astwarp --align rawimage.fits --output=aligned.fits ## Directly input a custom warping matrix (using fraction): $ astwarp --matrix=1/5,0,4/10,0,1/5,4/10,0,0,1 image.fits ## Directly input a custom warping matrix, with final numbers: $ astwarp --matrix="0.7071,-0.7071, 0.7071,0.7071" image.fits @end example If any processing is to be done, Warp can accept one file as input. As in all Gnuastro programs, when an output is not explicitly set with the @option{--output} option, the output filename will be set automatically based on the operation, see @ref{Automatic output}. For the full list of general options to all Gnuastro programs (including Warp), please see @ref{Common options}. To be the most accurate, the input image will be read as a 64-bit double precision floating point dataset and all internal processing is done in this format (including the raw output type). You can use the common @option{--type} option to write the output in any type you want, see @ref{Numeric data types}. Warps must be specified as command-line options, either as (possibly multiple) modular warpings (for example @option{--rotate}, or @option{--scale}), or directly as a single raw matrix (with @option{--matrix}). If specified together, the latter (direct matrix) will take precedence and all the modular warpings will be ignored. Any number of modular warpings can be specified on the command-line and configuration files. If more than one modular warping is given, all will be merged to create one warping matrix. As described in @ref{Merging multiple warpings}, matrix multiplication is not commutative, so the order of specifying the modular warpings on the command-line, and/or configuration files makes a difference (see @ref{Configuration file precedence}). The full list of modular warpings and the other options particular to Warp are described below. The values to the warping options (modular warpings as well as @option{--matrix}), are a sequence of at least one number. Each number in this sequence is separated from the next by a comma (@key{,}). Each number can also be written as a single fraction (with a forward-slash @key{/} between the numerator and denominator). Space and Tab characters are permitted between any two numbers, just don't forget to quote the whole value. Otherwise, the value will not be fully passed onto the option. See the examples above as a demonstration. @cindex FITS standard Based on the FITS standard, integer values are assigned to the center of a pixel and the coordinate [1.0, 1.0] is the center of the first pixel (bottom left of the image when viewed in SAO ds9). So the coordinate center [0.0, 0.0] is half a pixel away (in each axis) from the bottom left vertex of the first pixel. The resampling that is done in Warp (see @ref{Resampling}) is done on the coordinate axes and thus directly depends on the coordinate center. In some situations this if fine, for example when rotating/aligning a real image, all the edge pixels will be similarly affected. But in other situations (for example when scaling an over-sampled mock image to its intended resolution, this is not desired: you want the center of the coordinates to be on the corner of the pixel. In such cases, you can use the @option{--centeroncorner} option which will shift the center by @mymath{0.5} before the main warp, then shift it back by @mymath{-0.5} after the main warp, see below. @table @option @item -a @itemx --align Align the image and celestial (WCS) axes given in the input. After it, the vertical image direction (when viewed in SAO ds9) corresponds to the declination and the horizontal axis is the inverse of the Right Ascension (RA). The inverse of the RA is chosen so the image can correspond to what you would actually see on the sky and is common in most survey images. Align is internally treated just like a rotation (@option{--rotation}), but uses the input image's WCS to find the rotation angle. Thus, if you have rotated the image before calling @option{--align}, you might get unexpected results (because the rotation is defined on the original WCS). @item -r FLT @itemx --rotate=FLT Rotate the input image by the given angle in degrees: @mymath{\theta} in @ref{Warping basics}. Note that commonly, the WCS structure of the image is set such that the RA is the inverse of the image horizontal axis which increases towards the right in the FITS standard and as viewed by SAO ds9. So the default center for rotation is on the right of the image. If you want to rotate about other points, you have to translate the warping center first (with @option{--translate}) then apply your rotation and then return the center back to the original position (with another call to @option{--translate}, see @ref{Merging multiple warpings}. @item -s FLT[,FLT] @itemx --scale=FLT[,FLT] Scale the input image by the given factor(s): @mymath{M} and @mymath{N} in @ref{Warping basics}. If only one value is given, then both image axes will be scaled with the given value. When two values are given (separated by a comma), the first will be used to scale the first axis and the second will be used for the second axis. If you only need to scale one axis, use @option{1} for the axis you don't need to scale. The value(s) can also be written (on the command-line or in configuration files) as a fraction. @item -f FLT[,FLT] @itemx --flip=FLT[,FLT] Flip the input image around the given axis(s). If only one value is given, then both image axes are flipped. When two values are given (separated by a comma), you can choose which axis to flip over. @option{--flip} only takes values @code{0} (for no flip), or @code{1} (for a flip). Hence, if you want to flip by the second axis only, use @option{--flip=0,1}. @item -e FLT[,FLT] @itemx --shear=FLT[,FLT] Shear the input image by the given value(s): @mymath{A} and @mymath{B} in @ref{Warping basics}. If only one value is given, then both image axes will be sheared with the given value. When two values are given (separated by a comma), the first will be used to shear the first axis and the second will be used for the second axis. If you only need to shear along one axis, use @option{0} for the axis that must be untouched. The value(s) can also be written (on the command-line or in configuration files) as a fraction. @item -t FLT[,FLT] @itemx --translate=FLT[,FLT] Translate (move the center of coordinates) the input image by the given value(s): @mymath{c} and @mymath{f} in @ref{Warping basics}. If only one value is given, then both image axes will be translated by the given value. When two values are given (separated by a comma), the first will be used to translate the first axis and the second will be used for the second axis. If you only need to translate along one axis, use @option{0} for the axis that must be untouched. The value(s) can also be written (on the command-line or in configuration files) as a fraction. @item -p FLT[,FLT] @itemx --project=FLT[,FLT] Apply a projection to the input image by the given values(s): @mymath{g} and @mymath{h} in @ref{Warping basics}. If only one value is given, then projection will apply to both axes with the given value. When two values are given (separated by a comma), the first will be used to project the first axis and the second will be used for the second axis. If you only need to project along one axis, use @option{0} for the axis that must be untouched. The value(s) can also be written (on the command-line or in configuration files) as a fraction. @item -m STR @itemx --matrix=STR The warp/transformation matrix. All the elements in this matrix must be separated by comas(@key{,}) characters and as described above, you can also use fractions (a forward-slash between two numbers). The transformation matrix can be either a 2 by 2 (4 numbers), or a 3 by 3 (9 numbers) array. In the former case (if a 2 by 2 matrix is given), then it is put into a 3 by 3 matrix (see @ref{Warping basics}). @cindex NaN The determinant of the matrix has to be non-zero and it must not contain any non-number values (for example infinities or NaNs). The elements of the matrix have to be written row by row. So for the general Homography matrix of @ref{Warping basics}, it should be called with @command{--matrix=a,b,c,d,e,f,g,h,1}. The raw matrix takes precedence over all the modular warping options listed above, so if it is called with any number of modular warps, the latter are ignored. @item -c @itemx --centeroncorer Put the center of coordinates on the corner of the first (bottom-left when viewed in SAO ds9) pixel. This option is applied after the final warping matrix has been finalized: either through modular warpings or the raw matrix. See the explanation above for coordinates in the FITS standard to better understand this option and when it should be used. @item --hstartwcs=INT Specify the first header keyword number (line) that should be used to read the WCS information, see the full explanation in @ref{Invoking astcrop}. @item --hendwcs=INT Specify the last header keyword number (line) that should be used to read the WCS information, see the full explanation in @ref{Invoking astcrop}. @item -k @itemx --keepwcs @cindex WCSLIB @cindex World Coordinate System Do not correct the WCS information of the input image and save it untouched to the output image. By default the WCS (World Coordinate System) information of the input image is going to be corrected in the output image so the objects in the image are at the same WCS coordinates. But in some cases it might be useful to keep it unchanged (for example to correct alignments). @item -C FLT @itemx --coveredfrac=FLT Depending on the warp, the output pixels that cover pixels on the edge of the input image, or blank pixels in the input image, are not going to be fully covered by input data. With this option, you can specify the acceptable covered fraction of such pixels (any value between 0 and 1). If you only want output pixels that are fully covered by the input image area (and are not blank), then you can set @option{--coveredfrac=1}. Alternatively, a value of @code{0} will keep output pixels that are even infinitesimally covered by the input(so the sum of the pixels in the input and output images will be the same). @end table @node Data analysis, Modeling and fittings, Data manipulation, Top @chapter Data analysis Astronomical datasets (images or tables) contain very valuable information, the tools in this section can help in analyzing, extracting, and quantifying that information. For example getting general or specific statistics of the dataset (with @ref{Statistics}), detecting signal within a noisy dataset (with @ref{NoiseChisel}), or creating a catalog from an input dataset (with @ref{MakeCatalog}). @menu * Statistics:: Calculate dataset statistics. * NoiseChisel:: Detect objects in an image. * MakeCatalog:: Catalog from input and labeled images. * Match:: Match two datasets. @end menu @node Statistics, NoiseChisel, Data analysis, Data analysis @section Statistics The distribution of values in a dataset can provide valuable information about it. For example, in an image, if it is a positively skewed distribution, we can see that there is significant data in the image. If the distribution is roughly symmetric, we can tell that there is no significant data in the image. In a table, when we need to select a sample of objects, it is important to first get a general view of the whole sample. On the other hand, you might need to know certain statistical parameters of the dataset. For example, if we have run a detection algorithm on an image, and we want to see how accurate it was, one method is to calculate the average of the undetected pixels and see how reasonable it is (if detection is done correctly, the average of undetected pixels should be approximately equal to the background value, see @ref{Sky value}). In a table, you might have calculated the magnitudes of a certain class of objects and want to get some general characteristics of the distribution immediately on the command-line (very fast!), to possibly change some parameters. The Statistics program is designed for such situations. @menu * Histogram and Cumulative Frequency Plot:: Basic definitions. * Sigma clipping:: Definition of @mymath{\sigma}-clipping. * Sky value:: Definition and derivation of the Sky value. * Invoking aststatistics:: Arguments and options to Statistics. @end menu @node Histogram and Cumulative Frequency Plot, Sigma clipping, Statistics, Statistics @subsection Histogram and Cumulative Frequency Plot @cindex Histogram Histograms and the cumulative frequency plots are both used to visually study the distribution of a dataset. A histogram shows the number of data points which lie within pre-defined intervals (bins). So on the horizontal axis we have the bin centers and on the vertical, the number of points that are in that bin. You can use it to get a general view of the distribution: which values have been repeated the most? how close/far are the most significant bins? Are there more values in the larger part of the range of the dataset, or in the lower part? Similarly, many very important properties about the dataset can be deduced from a visual inspection of the histogram. In the Statistics program, the histogram can be either output to a table to plot with your favorite plotting program@footnote{We recommend @url{http://pgfplots.sourceforge.net/,PGFPlots} which generates your plots directly within @TeX{} (the same tool that generates your document).}, or it can be shown with ASCII characters on the command-line, which is very crude, but good enough for a fast and on-the-go analysis, see the example in @ref{Invoking aststatistics}. @cindex Intervals, histogram @cindex Bin width, histogram @cindex Normalizing histogram @cindex Probability density function The width of the bins is only necessary parameter for a histogram. In the limiting case that the bin-widths tend to zero (while assuming the number of points in the dataset tend to infinity), then the histogram will tend to the @url{https://en.wikipedia.org/wiki/Probability_density_function, probability density function} of the distribution. When the absolute number of points in each bin is not relevant to the study (only the shape of the histogram is important), you can @emph{normalize} a histogram so like the probability density function, the sum of all its bins will be one. @cindex Cumulative Frequency Plot In the cumulative frequency plot of a distribution, the horizontal axis is the sorted data values and the y axis is the index of each data in the sorted distribution. Unlike a histogram, a cumulative frequency plot does not involve intervals or bins. This makes it less prone to any sort of bias or error that a given bin-width would have on the analysis. When a larger number of the data points have roughly the same value, then the cumulative frequency plot will become steep in that vicinity. This occurs because on the horizontal axis, there is little change while on the vertical axis, the indexes constantly increase. Normalizing a cumulative frequency plot means to divide each index (y axis) by the total number of data points (or the last value). Unlike the histogram which has a limited number of bins, ideally the cumulative frequency plot should have one point for every data element. Even in small datasets (for example a @mymath{200\times200} image) this will result in an unreasonably large number of points to plot (40000)! As a result, for practical reasons, it is common to only store its value on a certain number of points (intervals) in the input range rather than the whole dataset, so you should determine the number of bins you want when asking for a cumulative frequency plot. In Gnuastro (and thus the Statistics program), the number reported for each bin is the total number of data points until the larger interval value for that bin. You can see an example histogram and cumulative frequency plot of a single dataset under the @option{--asciihist} and @option{--asciicfp} options of @ref{Invoking aststatistics}. So as a summary, both the histogram and cumulative frequency plot in Statistics will work with bins. Within each bin/interval, the lower value is considered to be within then bin (it is inclusive), but its larger value is not (it is exclusive). Formally, an interval/bin between a and b is represented by [a, b). When the over-all range of the dataset is specified (with the @option{--greaterequal}, @option{--lessthan}, or @option{--qrange} options), the acceptable values of the dataset are also defined with a similar inclusive-exclusive manner. But when the range is determined from the actual dataset (none of these options is called), the last element in the dataset is included in the last bin's count. @node Sigma clipping, Sky value, Histogram and Cumulative Frequency Plot, Statistics @subsection Sigma clipping Let's assume that you have pure noise (centered on zero) with a clear @url{https://en.wikipedia.org/wiki/Normal_distribution,Gaussian distribution}, or see @ref{Photon counting noise}. Now let's assume you add very bright objects (signal) on the image which have a very sharp boundary. By a sharp boundary, we mean that there is a clear cutoff (from the noise) at the pixels the objects finish. In other words, at their boundaries, the objects do not fade away into the noise. In such a case, when you plot the histogram (see @ref{Histogram and Cumulative Frequency Plot}) of the distribution, the pixels relating to those objects will be clearly separate from pixels that belong to parts of the image that did not have any signal (were just noise). In the cumulative frequency plot, after a steady rise (due to the noise), you would observe a long flat region were for a certain range of data (horizontal axis), there is no increase in the index (vertical axis). @cindex Blurring @cindex Cosmic rays @cindex Aperture blurring @cindex Atmosphere blurring Outliers like the example above can significantly bias the measurement of noise statistics. @mymath{\sigma}-clipping is defined as a way to avoid the effect of such outliers. In astronomical applications, cosmic rays (when they collide at a near normal incidence angle) are a very good example of such outliers. The tracks they leave behind in the image are perfectly immune to the blurring caused by the atmosphere and the aperture. They are also very energetic and so their borders are usually clearly separated from the surrounding noise. So @mymath{\sigma}-clipping is very useful in removing their effect on the data. See Figure 15 in Akhlaghi and Ichikawa, @url{https://arxiv.org/abs/1505.01664,2015}. @mymath{\sigma}-clipping is defined as the very simple iteration below. In each iteration, the range of input data might decrease and so when the outliers have the conditions above, the outliers will be removed through this iteration. The exit criteria will be discussed below. @enumerate @item Calculate the standard deviation (@mymath{\sigma}) and median (@mymath{m}) of a distribution. @item Remove all points that are smaller or larger than @mymath{m\pm\alpha\sigma}. @item Go back to step 1, unless the selected exit criteria is reached. @end enumerate @noindent The reason the median is used as a reference and not the mean is that the mean is too significantly affected by the presence of outliers, while the median is less affected, see @ref{Quantifying signal in a tile}. As you can tell from this algorithm, besides the condition above (that the signal have clear high signal to noise boundaries) @mymath{\sigma}-clipping is only useful when the signal does not cover more than half of the full data set. If they do, then the median will lie over the outliers and @mymath{\sigma}-clipping might remove the pixels with no signal. There are commonly two exit criteria to stop the @mymath{\sigma}-clipping iteration: @itemize @item When a certain number of iterations has taken place (second value to the @option{--sigclip} option is larger than 1). @item When the new measured standard deviation is within a certain tolerance level of the old one (second value to the @option{--sigclip} option is less than 1). The tolerance level is defined by: @dispmath{\sigma_{old}-\sigma_{new} \over \sigma_{new}} The standard deviation is used because it is heavily influenced by the presence of outliers. Therefore the fact that it stops changing between two iterations is a sign that we have successfully removed outliers. Note that in each clipping, the dispersion in the distribution is either less or equal. So @mymath{\sigma_{old}\geq\sigma_{new}}. @end itemize @cartouche @noindent When working on astronomical images, objects like galaxies and stars are blurred by the atmosphere and the telescope aperture, therefore their signal sinks into the noise very gradually. Galaxies in particular do not appear to have a clear high signal to noise cutoff at all. Therefore @mymath{\sigma}-clipping will not be useful in removing their effect on the data. To gauge if @mymath{\sigma}-clipping will be useful for your dataset, look at the histogram (see @ref{Histogram and Cumulative Frequency Plot}). The ASCII histogram that is printed on the command-line with @option{--asciihist} is good enough in most cases. @end cartouche @node Sky value, Invoking aststatistics, Sigma clipping, Statistics @subsection Sky value @cindex Sky One of the most important aspects of a dataset is its reference value: the value of the dataset where there is no signal. Without knowing, and thus removing the effect of, this value it is impossible to compare the derived results of many high-level analyses over the dataset with other datasets (in the attempt to associate our results with the ``real'' world). In astronomy, this reference value is known as the ``Sky'' value: the value where there is no signal from objects (for example galaxies, stars, planets or comets). Depending on the dataset, the Sky value maybe a fixed value over the whole dataset, or it may vary based on location. For an example of the latter case, see Figure 11 in @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa (2015)}. Because of the significance of the Sky value in astronomical data analysis, we have devoted this subsection to it for a thorough review. We start with a thorough discussion on its definition (@ref{Sky value definition}). In the astronomical literature, researchers use a variety of methods to estimate the Sky value, so in @ref{Sky value misconceptions}) we review those and discuss their biases. From the definition of the Sky value, the most accurate way to estimate the Sky value is to run a detection algorithm (for example @ref{NoiseChisel}) over the dataset and use the un-detected pixels. However, there is also a more crude method that maybe useful when good direct detection is not initially possible (for example due to too many cosmic rays in a shallow image). A more crude (but simpler method) that is usable in such situations is discussed in @ref{Quantifying signal in a tile}. @menu * Sky value definition:: Definition of the Sky/reference value. * Sky value misconceptions:: Wrong methods to estimate the Sky value. * Quantifying signal in a tile:: Method to estimate the presence of signal. @end menu @node Sky value definition, Sky value misconceptions, Sky value, Sky value @subsubsection Sky value definition @cindex Sky value This analysis is taken from @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa (2015)}. Let's assume that all instrument defects -- bias, dark and flat -- have been corrected and the brightness (see @ref{Flux Brightness and magnitude}) of a detected object, @mymath{O}, is desired. The sources of flux on pixel @mymath{i}@footnote{For this analysis the dimension of the data (image) is irrelevant. So if the data is an image (2D) with width of @mymath{w} pixels, then a pixel located on column @mymath{x} and row @mymath{y} (where all counting starts from zero and (0, 0) is located on the bottom left corner of the image), would have an index: @mymath{i=x+y\times{}w}.} of the image can be written as follows: @itemize @item Contribution from the target object, (@mymath{O_i}). @item Contribution from other detected objects, (@mymath{D_i}). @item Undetected objects or the fainter undetected regions of bright objects, (@mymath{U_i}). @item @cindex Cosmic rays A cosmic ray, (@mymath{C_i}). @item @cindex Background flux The background flux, which is defined to be the count if none of the others exists on that pixel, (@mymath{B_i}). @end itemize @noindent The total flux in this pixel (@mymath{T_i}) can thus be written as: @dispmath{T_i=B_i+D_i+U_i+C_i+O_i.} @cindex Cosmic ray removal @noindent By definition, @mymath{D_i} is detected and it can be assumed that it is correctly estimated (deblended) and subtracted, thus @mymath{D_i=0}. There are also methods to detect and remove cosmic rays, for example the method described in van Dokkum (2001)@footnote{van Dokkum, P. G. (2001). Publications of the Astronomical Society of the Pacific. 113, 1420.}, or by comparing multiple exposures. This allows us to set @mymath{C_i=0}. Note that in practice, @mymath{D_i} and @mymath{U_i} are correlated, because they both directly depend on the detection algorithm and its input parameters. Also note that no detection or cosmic ray removal algorithm is perfect. With these limitations in mind, the observed Sky value for this pixel (@mymath{S_i}) can be defined as @cindex Sky value @dispmath{S_i=B_i+U_i.} @noindent Therefore, as the detection process (algorithm and input parameters) becomes more accurate, or @mymath{U_i\to0}, the sky value will tend to the background value or @mymath{S_i\to B_i}. Therefore, while @mymath{B_i} is an inherent property of the data (pixel in an image), @mymath{S_i} depends on the detection process. Over a group of pixels, for example in an image or part of an image, this equation translates to the average of undetected pixels. With this definition of sky, the object flux in the data can be calculated with @dispmath{ T_{i}=S_{i}+O_{i} \quad\rightarrow\quad O_{i}=T_{i}-S_{i}.} @noindent @cindex photo-electrons Hence, the more accurately @mymath{S_i} is measured, the more accurately the brightness (sum of pixel values) of the target object can be measured (photometry). Any under-(over-)estimation in the sky will directly translate to an over-(under-)estimation of the measured object's brightness. In the fainter outskirts of an object a very small fraction of the photo-electrons in the pixels actually belong to objects (see Figure 1b in @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa (2015)}). Therefore even a small over estimation of the sky value will result in the loss of a very large portion of most galaxies. Besides the lost area/brightness, this will also cause an over-estimation of the Sky value and thus even more under-estimation of the object's brightness. It is thus very important to detect the diffuse flux of a target, even if they are not your primary target. @cartouche @noindent The @strong{Sky value} is only correctly found when all the detected objects (@mymath{D_i} and @mymath{C_i}) have been removed from the data. @end cartouche @node Sky value misconceptions, Quantifying signal in a tile, Sky value definition, Sky value @subsubsection Sky value misconceptions As defined in @ref{Sky value}, the sky value is only accurately defined when the detection algorithm is not significantly reliant on the sky value. In particular its detection threshold. However, most signal-based detection tools@footnote{According to Akhlaghi and Ichikawa (2015), signal-based detection is a detection process that relies heavily on assumptions about the to-be-detected objects. This method was the most heavily used technique prior to the introduction of NoiseChisel in that paper.} use the sky value as a reference to define the detection threshold. So these old techniques had to rely on approximations based on other assumptions about the data. A review of those other techniques can be seen in Appendix A of Akhlaghi and Ichikawa (2015)@footnote{Akhlaghi M., Ichikawa. T. (2015). Astrophysical Journal Supplement Series.}. Since they were extensively used in astronomical data analysis for several decades, such approximations have given rise to a lot of misconceptions, ambiguities and disagreements about the sky value and how to measure it. As a summary, the major methods used until now were an approximation of the mode of the image pixel distribution and @mymath{\sigma}-clipping. @itemize @cindex Histogram @cindex Distribution mode @cindex Mode of a distribution @cindex Probability density function @item To find the mode of a distribution those methods would either have to assume (or find) a certain probability density function (PDF) or use the histogram. But astronomical datasets can have any distribution, making it almost impossible to define a generic function. Also, histogram-based results are very inaccurate (there is a large dispersion) and it depends on the histogram bin-widths. @cindex sigma-clipping @item Another approach was to iteratively clip the brightest pixels in the image (which is known as @mymath{\sigma}-clipping, since the reference was found from the image mean and its standard deviation or @mymath{\sigma}). See @ref{Sigma clipping} for a complete explanation. The problem with @mymath{\sigma}-clipping was that real astronomical objects have diffuse and faint wings that penetrate deeply into the noise. So only removing their brightest parts is completely useless in removing the systematic bias an object's fainter parts cause in the sky value. @end itemize As discussed in @ref{Sky value}, the sky value can only be correctly defined as the average of undetected pixels. Therefore all such approaches that try to approximate the sky value prior to detection are ultimately poor approximations. @node Quantifying signal in a tile, , Sky value misconceptions, Sky value @subsubsection Quantifying signal in a tile @cindex Data @cindex Noise @cindex Signal @cindex Gaussian distribution Put simply, noise can characterized with a certain spread about a characteristic value. In the Gaussian distribution (most commonly used to model noise) the spread is defined by the standard deviation about the characteristic mean. Before continuing let's clarify some definitions first: @emph{Data} is defined as the combination of signal and noise (so a noisy image is one @emph{data}-set). @emph{Signal} is defined as the mean of the noise on each element (after sky subtraction, see @ref{Sky value definition}). Let's assume that the @emph{background} (see @ref{Sky value definition}) is subtracted and is zero. When a data set doesn't have any signal (only noise), the mean, median and mode of the distribution are equal within statistical errors and approximately equal to the background value. Signal always has a positive value and will never become negative, see Figure 1 in @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa (2015)}. Therefore, as more signal is added to the raw noise, the mean, median and mode of the dataset (which has both signal and noise) shift to the positive. The mean's shift is the largest. The median shifts less, since it is defined based on an ordered distribution and so is not affected by a small number of outliers. The distribution's mode shifts the least to the positive. @cindex Mode @cindex Median Inverting the argument above gives us a robust method to quantify the significance of signal in a dataset. Namely, when the mode and median of a distribution are approximately equal, we can argue that there is no significant signal. To allow for gradients (which are commonly present in ground-based images), we can consider the image to be made of a grid of tiles (see @ref{Tessellation}@footnote{The options to customize the tessellation are discussed in @ref{Processing options}.}). Hence, from the difference of the mode and median on each tile, we can `detect' the significance of signal in it. The median of a distribution is defined to be the value of the distribution's middle point after sorting (or 0.5 quantile). Thus, to estimate the presence of signal, we'll compare with the quantile of the mode with 0.5, if the difference is larger than the value given to the @option{--modmedqdiff} option, this tile will be ignored. You can read this option as ``mode-median-quantile-diff''. This method to use the input's skewness is possible because of a new algorithm to find the mode of a distribution that was defined in Appendix C of Akhlaghi and Ichikawa (2015). However, the raw dataset's distribution is noisy (noise also affects the sorting), so using the argument above on the raw input will give a noisy result. To decrease the noise/error in estimating the mode, we will use convolution (see @ref{Convolution process}). Convolution decreases the range of the dataset and enhances its skewness, See Section 3.1.1 and Figure 4 in Akhlaghi and Ichikawa (2015). This enhanced skewness can be interpreted as an increase in the Signal to noise ratio of the objects buried in the noise. Therefore, to obtain an even better measure of the presence of signal in a mesh, the image can be convolved with a given kernel first. Note that through the difference of the mode and median we have actually `detected' data in the distribution. However this ``detection'' was only based on the total distribution of the data in each tile (a much lower resolution). This is the main limitation of this technique. The best approach is thus to do detection over the dataset, mask all the detected pixels and use the undetected regions to estimate the sky and its standard deviation. @cindex Cosmic rays The mean value of the tiles that have an approximately equal mode and median will be the Sky value. However there is one final hurdle: astronomical datasets are commonly plagued with Cosmic rays. Images of Cosmic rays aren't smoothed by the atmosphere or telescope aperture, so they have sharp boundaries. Also, since they don't occupy too many pixels, they don't affect the mode and median calculation. But their very high values can greatly bias the calculation of the mean (recall how the mean shifts the fastest in the presence of outliers), see Figure 15 in Akhlaghi and Ichikawa (2015) for one example. The effect of outliers like cosmic rays on the mean and standard deviation can be removed through @mymath{\sigma}-clipping, see @ref{Sigma clipping} for a complete explanation. Therefore, after asserting that the mode and median are approximately equal in a tile (see @ref{Tessellation}), the final Sky value and its standard deviation are determined after @mymath{\sigma}-clipping with the @option{--sigmaclip} option. @node Invoking aststatistics, , Sky value, Statistics @subsection Invoking Statistics Statistics will print statistical measures of an input dataset (table column or image). The executable name is @file{aststatistics} with the following general template @example $ aststatistics [OPTION ...] InputImage.fits @end example @noindent One line examples: @example ## Print some general statistics of input image: $ aststatistics image.fits ## Print some general statistics of column named MAG_F160W: $ aststatistics catalog.fits -h1 --column=MAG_F160W ## Make the histogram of the column named MAG_F160W: $ aststatistics table.fits -cMAG_F160W --histogram ## Find the Sky value on image with a given kernel: $ aststatistics image.fits --sky --kernel=kernel.fits ## Print Sigma-clipped results of records with a MAG_F160W ## column value between 26 and 27: $ aststatistics cat.fits -cMAG_F160W -g26 -l27 --sigmaclip=3,0.2 ## Print the median value of all records in column MAG_F160W that ## have a value larger than 3 in column PHOTO_Z: $ aststatistics tab.txt -rPHOTO_Z -g3 -cMAG_F160W --median @end example @noindent An input image or table is necessary when processing is to be done. If any output file is to be created, the value to the @option{--output} option, is used as the base name for the generated files. Without @option{--output}, the input name will be used to generate an output name, see @ref{Automatic output}. The options described below are particular to Statistics, but for general operations, it shares a large collection of options with the other Gnuastro programs, see @ref{Common options} for the full list. Options can also be given in configuration files, for more, please see @ref{Configuration files}. The input dataset may have blank values (see @ref{Blank pixels}), in this case, all blank pixels are ignored during the calculation. Initially, the full dataset will be read, but it is possible to select a specific range of data elements to use in the analysis of each run. You can either directly specify a minimum and maximum value for the range of data elements to use (with @option{--greaterequal} or @option{--lessthan}), or specify the range using quantiles (with @option{--qrange}). If a range is specified, all pixels outside of it are ignored before any processing. The following set of options are for specifying the input/outputs of Statistics. There are many other input/output options that are common to all Gnuastro programs including Statistics, see @ref{Input output options} for those. @table @option @item -c STR/INT @itemx --column=STR/INT The input column selector when the input file is a table. See @ref{Selecting table columns} for a full description of how to use this option. For more on how tables are read in Gnuastro, please see @ref{Tables}. @item -r STR/INT @itemx --refcol=STR/INT The reference column selector when the input file is a table. When a reference column is given, the range options below will be applied to this column and only elements in the input column that have a reference value in the correct range will be used. In practice this option allows you to select a subset of the input column based on values in another (the reference) column. All the statistical calculations will be done on the selected input column, not the reference column. @item -g FLT @itemx --greaterequal=FLT Limit the range of inputs into those with values greater and equal to what is given to this option. None of the values below this value will be used in any of the processing steps below. @item -l FLT @itemx --lessthan=FLT Limit the range of inputs into those with values less-than what is given to this option. None of the values greater or equal to this value will be used in any of the processing steps below. @item -Q FLT[,FLT] @itemx --qrange=FLT[,FLT] Specify the range of usable inputs using the quantile. This option can take one or two quantiles to specify the range. When only one number is input (let's call it @mymath{Q}), the range will be those values in the quantile range @mymath{Q} to @mymath{1-Q}. So when only one value is given, it must be less than 0.5. When two values are given, the first is used as the lower quantile range and the second is used as the larger quantile range. @cindex Quantile The quantile of a given element in a dataset is defined by the fraction of its index to the total number of values in the sorted input array. So the smallest and largest values in the dataset have a quantile of 0.0 and 1.0. The quantile is a very useful non-parametric (making no assumptions about the input) relative measure to specify a range. It can best be understood in terms of the cumulative frequency plot, see @ref{Histogram and Cumulative Frequency Plot}. The quantile of each horizontal axis value in the cumulative frequency plot is the vertical axis value associate with it. @end table @cindex ASCII plot When no operation is requested, Statistics will print some general basic properties of the input dataset on the command-line like the example below (ran on one of the output images of @command{make check}@footnote{You can try it by running the command in the @file{tests} directory, open the image with a FITS viewer and have a look at it to get a sense of how these statistics relate to the input image/dataset.}). This default behavior is designed to help give you a general feeling of how the data are distributed and help in narrowing down your analysis. @example $ aststatistics convolve_spatial_scaled_noised.fits \ --greaterequal=9500 --lessthan=11000 Statistics (GNU Astronomy Utilities) X.X ------- Input: convolve_spatial_scaled_noised.fits (hdu: 0) Range: from (inclusive) 9500, upto (exclusive) 11000. Unit: Brightness ------- Number of elements: 9074 Minimum: 9622.35 Maximum: 10999.7 Mode: 10055.45996 Mode quantile: 0.4001983908 Median: 10093.7 Mean: 10143.98257 Standard deviation: 221.80834 ------- Histogram: | ** | ****** | ******* | ********* | ************* | ************** | ****************** | ******************** | *************************** * | ***************************************** *** |* ************************************************************** |----------------------------------------------------------------- @end example Gnuastro's Statistics is a very general purpose program, so to be able to easily understand this diversity in its operations (and how to possibly run them together), we'll divided the operations into two types: those that don't respect the position of the elements and those that do (by tessellating the input on a tile grid, see @ref{Tessellation}). The former treat the whole dataset as one and can re-arrange all the elements (for example sort them), but the former do their processing on each tile independently. First, we'll review the operations that work on the whole dataset. @cindex AWK @cindex GNU AWK The group of options below can used to get a single value measurement of the whole dataset. They will print only the requested value as one field in a line/row, like the @option{--mean}, @option{--median} options. These options can be called any number of times and in any order. The outputs of all such options will be printed on one line following each other (with a space character between them). This feature makes these options very useful in scripts, or to redirect into programs like GNU AWK for higher-level processing. These are some of the most basic measures, Gnuastro is still under heavy development and this list will grow. If you want another statistical parameter, please contact us and we will do out best to add it to this list, see @ref{Suggest new feature}. @table @option @item -n @itemx --number Print the number of all used (non-blank and in range) elements. @item --minimum Print the minimum value of all used elements. @item --maximum Print the maximum value of all used elements. @item --sum Print the sum of all used elements. @item -m @itemx --mean Print the mean (average) of all used elements. @item -t @itemx --std Print the standard deviation of all used elements. @item -E @itemx --median Print the median of all used elements. @item -u FLT[,FLT[,...]] @itemx --quantile=FLT[,FLT[,...]] Print the values at the given quantiles of the input dataset. Any number of quantiles may be given and one number will be printed for each. Values can either be written as a single number or as fractions, but must be between zero and one (inclusive). Hence, in effect @command{--quantile=0.25 --quantile=0.75} is equivalent to @option{--quantile=0.25,3/4}, or @option{-u1/4,3/4}. The returned value is one of the elements from the dataset. Taking @mymath{q} to be your desired quantile, and @mymath{N} to be the total number of used (non-blank and within the given range) elements, the returned value is at the following position in the sorted array: @mymath{round(q\times{}N}). @item --quantfunc=FLT[,FLT[,...]] Print the quantiles of the given values in the dataset. This option is the inverse of the @option{--quantile} and operates similarly except that the acceptable values are within the range of the dataset, not between 0 and 1. Formally it is known as the ``Quantile function''. Since the dataset is not continuous this function will find the nearest element of the dataset and use its position to estimate the quantile function. @item -O @itemx --mode Print the mode of all used elements. The mode is found through the mirror distribution which is fully described in Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015}. See that section for a full description. This mode calculation algorithm is non-parametric, so when the dataset is not large enough (larger than about 1000 elements usually), or doesn't have a clear mode it can fail. In such cases, this option will return a value of @code{nan} (for the floating point NaN value). As described in that paper, the easiest way to assess the quality of this mode calculation method is to use it's symmetricity (see @option{--modesym} below). A better way would be to use the @option{--mirror} option to generate the histogram and cumulative frequency tables for any given mirror value (the mode in this case) as a table. If you generate plots like those shown in Figure 21 of that paper, then your mode is accurate. @item --modequant Print the quantile of the mode. You can get the actual mode value from the @option{--mode} described above. In many cases, the absolute value of the mode is irrelevant, but its position within the distribution is important. In such cases, this option will become handy. @item --modesym Print the symmetricity of the calculated mode. See the description of @option{--mode} for more. This mode algorithm finds the mode based on how symmetric it is, so if the symmetricity returned by this option is too low, the mode is not too accurate. See Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015} for a full description. In practice, symmetricity values larger than 0.2 are mostly good. @item --modesymvalue Print the value in the distribution where the mirror and input distributions are no longer symmetric, see @option{--mode} and Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015} for more. @end table The list of options below are for those statistical operations that output more than one value. So while they can be called together in one run, their outputs will be distinct (each one's output will usually be printed in more than one line). @table @option @item -A @itemx --asciihist Print an ASCII histogram of the usable values within the input dataset along with some basic information like the example below (from the UVUDF catalog@footnote{@url{https://asd.gsfc.nasa.gov/UVUDF/uvudf_rafelski_2015.fits.gz}}). The width and height of the histogram (in units of character widths and heights on your command-line terminal) can be set with the @option{--numasciibins} (for the width) and @option{--asciiheight} options. For a full description of the histogram, please see @ref{Histogram and Cumulative Frequency Plot}. An ASCII plot is certainly very crude and cannot be used in any publication, but it is very useful for getting a general feeling of the input dataset very fast and easily on the command-line without having to take your hands off the keyboard (which is a major distraction!). If you want to try it out, you can write it all in one line and ignore the @key{\} and extra spaces. @example $ aststatistics uvudf_rafelski_2015.fits.gz --hdu=1 \ --column=MAG_F160W --lessthan=40 \ --asciihist --numasciibins=55 ASCII Histogram: Number: 8593 Y: (linear: 0 to 660) X: (linear: 17.7735 -- 31.4679, in 55 bins) | **** | ***** | ****** | ******** | ********* | *********** | ************** | ***************** | *********************** | ******************************** |*** *************************************************** |------------------------------------------------------- @end example @item --asciicfp Print the cumulative frequency plot of the usable elements in the input dataset. Please see descriptions under @option{--asciihist} for more, the example below is from the same input table as that example. To better understand the cumulative frequency plot, please see @ref{Histogram and Cumulative Frequency Plot}. @example $ aststatistics uvudf_rafelski_2015.fits.gz --hdu=1 \ --column=MAG_F160W --lessthan=40 \ --asciicfp --numasciibins=55 ASCII Cumulative frequency plot: Y: (linear: 0 to 8593) X: (linear: 17.7735 -- 31.4679, in 55 bins) | ******* | ********** | *********** | ************* | ************** | *************** | ***************** | ******************* | *********************** | ****************************** |******************************************************* |------------------------------------------------------- @end example @item -H @itemx --histogram Save the histogram of the usable values in the input dataset into a table. The first column is the value at the center of the bin and the second is the number of points in that bin. If the @option{--cumulative} option is also called with this option in a run, then the table will have three columns (the third is the cumulative frequency plot). Through the @option{--numbins} and @option{--lowerbin} you can modify the first column values and with @option{--normalize} and @option{--maxbinone} you can modify the second columns. See below for the description of each. By default (when no @option{--output} is specified) a plain text table will be created, see @ref{Gnuastro text table format}. If a FITS name is specified, you can use the common option @option{--tableformat} to have it as a FITS ASCII or FITS binary format, see @ref{Common options}. This table can then be fed into your favorite plotting tool and get a much more clean and nice histogram than what the raw command-line can offer you (with the @option{--asciihist} option). @item -C @itemx --cumulative Save the cumulative frequency plot of the usable values in the input dataset into a table, similar to @option{--histogram}. @item -s @itemx --sigmaclip Do @mymath{\sigma}-clipping on the usable pixels of the input dataset. See @ref{Sigma clipping} for a full description on @mymath{\sigma}-clipping and also to better understand this option. The @mymath{\sigma}-clipping parameters can be set through the @option{--sclipparams} option (see below). @item --mirror=FLT Make a histogram and cumulative frequency plot of the mirror distribution for the given dataset when the mirror is located at the value to this option. The mirror distribution is fully described in Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015} and currently it is only used to calculate the mode (see @option{--mode}). Just note that the mirror distribution is a discrete distribution like the input, so while you may give any number as the value to this option, the actual mirror value is the closest number in the input dataset to this value. If the two numbers are different, Statistics will warn you of the actual mirror value used. This option will make a table as output. Depending on your selected name for the output, it will be either a FITS table or a plain text table (which is the default). It contains three columns: the first is the center of the bins, the second is the histogram (with the largest value set to 1) and the third is the normalized cumulative frequency plot of the mirror distribution. The bins will be positioned such that the mode is on the starting interval of one of the bins to make it symmetric around the mirror. With this output file and the input histogram (that you can generate in another run of Statistics, using the @option{--onebinvalue}), it is possible to make plots like Figure 21 of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015}. @end table The list of options below allow customization of the histogram and cumulative frequency plots (for the @option{--histogram}, @option{--cumulative}, @option{--asciihist}, and @option{--asciicfp} options). @table @option @item --numbins The number of bins (rows) to use in the histogram and the cumulative frequency plot tables (outputs of @option{--histogram} and @option{--cumulative}). @item --numasciibins The number of bins (characters) to use in the ASCII plots when printing the histogram and the cumulative frequency plot (outputs of @option{--asciihist} and @option{--asciicfp}). @item --asciiheight The number of lines to use when printing the ASCII histogram and cumulative frequency plot on the command-line (outputs of @option{--asciihist} and @option{--asciicfp}). @item -n @itemx --normalize Normalize the histogram or cumulative frequency plot tables (outputs of @option{--histogram} and @option{--cumulative}). For a histogram, the sum of all bins will become one and for a cumulative frequency plot the last bin value will be one. @item --maxbinone Divide all the histogram values by the maximum bin value so it becomes one and the rest are similarly scaled. In some situations (for example if you want to plot the histogram and cumulative frequency plot in one plot) this can be very useful. @item --onebinstart=FLT Make sure that one bin starts with the value to this option. In practice, this will shift the bins used to find the histogram and cumulative frequency plot such that one bin's lower interval becomes this value. For example when the histogram range includes negative and positive values and zero has a special significance in your analysis, then zero will be somewhere in one bin and will mix counts of positive and negative. By setting @option{--onebinstart=0}, you can make sure that the viewers of the histogram will not be confused without doing the math of setting a range and number of bins. @cindex NaN Note that by default, the first row of the histogram and cumulative frequency plot show the central values of each bin. So in the example above you will not see the 0.000 in the first column, you will see two symmetric values. If the value is not within the usable input range, this option will be ignored. @end table All the options described until now were from the first class of operations discussed above: those that treat the whole dataset as one. However. It often happens that the relative position of the dataset elements over the dataset is significant. For example you don't want one median value for the whole input image, you want to know how the median changes over the image. For such operations, the input has to be tessellated (see @ref{Tessellation}). Thus this class of options can't currently be called along with the options above in one run of Statistics. @table @option @item -t @itemx --ontile Do the respective single-valued calculation over one tile of the input dataset, not the whole dataset. This option must be called with at least one of the single valued options discussed above (for example @option{--mean} or @option{--quantile}). The output will be a file in the same format as the input. If the @option{--oneelempertile} option is called, then one element/pixel will be used for each tile (see @ref{Processing options}). Otherwise, the output will have the same size as the input, but each element will have the value corresponding to that tile's value. If multiple single valued operations are called, then for each operation there will be one extension in the output FITS file. @item -y @itemx --sky Estimate the Sky value on each tile as fully described in @ref{Quantifying signal in a tile}. As described in that section, several options are necessary to configure the Sky estimation which are listed below. The output file will have two extensions: the first is the Sky value and the second is the Sky standard deviation on each tile. Similar to @option{--ontile}, if the @option{--oneelempertile} option is called, then one element/pixel will be used for each tile (see @ref{Processing options}). @end table The parameters for estimating the sky value can be set with the following options, except for the @option{--sclipparams} option (which is also used by the @option{--sigmaclip}), the rest are only used for the Sky value estimation. @table @option @item -k=STR @itemx --kernel=STR File name of kernel to help in estimating the significance of signal in a tile, see @ref{Quantifying signal in a tile}. @item --khdu=STR Kernel HDU to help in estimating the significance of signal in a tile, see @ref{Quantifying signal in a tile}. @item --mirrordist=FLT Maximum distance (as a multiple of error) to estimate the difference between the input and mirror distributions in finding the mode, see Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015}, also see @ref{Quantifying signal in a tile}. @item --modmedqdiff=FLT The maximum acceptable distance between the mode and median, see @ref{Quantifying signal in a tile}. @item --sclipparams=FLT,FLT The @mymath{\sigma}-clipping parameters, see @ref{Sigma clipping}. This option takes two values which are separated by a comma (@key{,}). Each value can either be written as a single number or as a fraction of two numbers (for example @code{3,1/10}). The first value to this option is the multiple of @mymath{\sigma} that will be clipped (@mymath{\alpha} in that section). The second value is the exit criteria. If it is less than 1, then it is interpreted as tolerance and if it is larger than one it is a specific number. Hence, in the latter case the value must be an integer. @item --smoothwidth=INT Width of a flat kernel to convolve the interpolated tile values. Tile interpolation is done using the median of the @option{--interpnumngb} neighbors of each tile (see @ref{Processing options}). If this option is given a value of zero or one, no smoothing will be done. Without smoothing, strong boundaries will probably be created between the values estimated for each tile. It is thus good to smooth the interpolated image so strong discontinuities do not show up in the final Sky values. The smoothing is done through convolution (see @ref{Convolution process}) with a flat kernel, so the value to this option must be an odd number. @item --checksky Create a multi-extension FITS file showing the steps that were used to estimate the Sky value over the input, see @ref{Quantifying signal in a tile}. The file will have two extensions for each step (one for the Sky and one for the Sky standard deviation). @end table @node NoiseChisel, MakeCatalog, Statistics, Data analysis @section NoiseChisel @cindex Labeling @cindex Detection @cindex Segmentation Once instrumental signatures are removed from the raw data in the initial reduction process (see @ref{Data manipulation}). We are ready to derive scientific results out of them. But we can't do anything special with a raw dataset, for example an image is just an array of values. Every pixel just has one value and its position within the image. Therefore, the first step of your high-level analysis will be to classify/label the dataset elements/pixels into two classes: signal and noise. This process is formally known as @emph{detection}. Afterwards, you want to separate the detections into multiple components (for example when two detected regions aren't touching, they should be treated independently as two distant galaxies for example). This higher level classification of the detections is known as @emph{segmentation}. NoiseChisel is Gnuastro's program for detection and segmentation. NoiseChisel works based on a new noise-based approach to signal detection and was introduced to the astronomical community in @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]}. NoiseChisel's primary output is an array (image) with the same size as the input but containing labels: those pixels with a label of 0 are noise/sky while those pixels with labels larger than 0 are detections (separate segments will be given positive integers, starting from 1). For more on NoiseChisel's particular output format and its benefits (especially in conjunction with @ref{MakeCatalog}), please see @url{https://arxiv.org/abs/1611.06387, Akhlaghi [2016]}. The published paper cannot under go any updates, but the NoiseChisel software has evolved, you can see the major changes in @ref{NoiseChisel changes after publication}. Data is inherently mixed with noise: only mock/simulated datasets are free of noise. So this process of separating signal from noise is not trivial. In particular, most scientifically interesting astronomical targets are faint, can have a large variety of morphologies along with a large distribution in brightness and size which are all drowned in a ocean of noise. So detection is a uniquely vital aspect of any scientific work and even more so for astronomical research. This is such a fundamental step that designing of NoiseChisel was the primary motivation behind creating Gnuastro: the first generation of Gnuastro's programs were all first part of what later became NoiseChisel, afterwards they spinned-off into separate programs. @cindex Erosion The name of NoiseChisel is derived from the first thing it does after thresholding the dataset: to erode it. In mathematical morphology, erosion on pixels can be pictured as carving off boundary pixels. Hence, what NoiseChisel does is similar to what a wood chisel or stone chisel do. It is just not a hardware, but a software. In fact looking at it as a chisel and your dataset as a solid cube of rock will greatly help in best using it: with NoiseChisel you literally carve the galaxies/stars/comets out of the noise. Try running it with the @option{--checkdetection} option to see each step of the carving process on your input dataset. You can then change a specific option to carve out your signal out of the noise more successfully. @menu * NoiseChisel changes after publication:: Changes to the software after publication. * Invoking astnoisechisel:: Options and arguments for NoiseChisel. @end menu @node NoiseChisel changes after publication, Invoking astnoisechisel, NoiseChisel, NoiseChisel @subsection NoiseChisel changes after publication Before using NoiseChisel it is strongly recommended to read @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]} to gain a good understanding of what it does and how each parameter influences the output. Thanks to that paper, there is no need to go into the details of the major processing steps. Hence we can just dive into the details of running NoiseChisel in @ref{Invoking astnoisechisel}. However, the paper cannot undergo any further updates, but NoiseChisel will evolve: better algorithms or steps will be found, thus options will be added or removed. So this book is the final and definitive guide. For a more detailed list of changes in each release, please follow the @file{NEWS} file. The @file{NEWS} file is in the released Gnuastro tarball (see @ref{Release tarball}). You can also view the most recent @file{NEWS} file @url{http://git.savannah.gnu.org/cgit/gnuastro.git/plain/NEWS, online}@footnote{The online version of the @file{NEWS} file here may contain features that have been implemented, but not yet officially released as a tarball (see @ref{Downloading the source}). Therefore, please be sure to look at the dates and versions above each group of changed features and make sure it corresponds to your installed version. It is hence recommended to always stay up to date, see @ref{Announcements}).}. To make the transition form the paper to this book easier (and encourage reading the paper), below you can see the major changes since the paper was published. First, the options that have been removed are discussed, followed by those that have been added. @noindent Removed options: @itemize @item @option{--dilate}: In the paper, true detections were dilated for a final dig into the noise. However, simple 8-connected dilation can produce boxy results which are not realistic and could miss diffuse flux. The final dig into the noise is now done by ``grow''ing the true detections, similar to how true clumps were grown, see the description of @option{--detgrowquant} below and in @ref{Detection options} for more on the new alternative. @end itemize @noindent Added options: @itemize @item @option{--widekernel}: NoiseChisel uses the difference between the mode and median to identify if a tile should be used for estimating the quantile thresholds (see @ref{Quantifying signal in a tile}). Until now, NoiseChisel would convolve an image once and estimate the proper tiles for quantile estimations on the convolved image. The same convolved image would later be used for quantile estimation. A larger kernel does increase the skewness (and thus difference between the mode and median), however, it disfigures the shapes/morphology of the objects. This new @option{--widekernel} option (and a corresponding @option{--wkhdu} option to specify its HDU) option are added to solve such cases. When its given, the input will be convolved with both the sharp (given through the @option{--kernel} option) and wide kernels. The mode and median are calculated on the dataset that is convolved with the wider kernel, then the quantiles are estimated on the image convolved with the sharper kernel. @item @option{--noerodequant}: to specify a quantile threshold where erosion will not apply. This is useful to detect sharper point-like sources that will be missed due to too much erosion. To completely ignore this features give this option a value of 1 (only the largest valued pixel in the input will not be eroded). @item @option{--qthreshtilequant}: to manually remove the measured qthresh from some tiles. This feature helps in detecting large and extended diffuse (almost flat) signal when necessary, see @ref{Detection options}. @item @option{--detgrowquant}: is used to grow the final true detections until a given quantile in the same way that clumps are grown during segmentation (compare columns 2 and 3 in Figure 10 of the paper). It replaces the old @option{--dilate} option in the paper and older versions of Gnuastro. Dilation is a blind growth method which causes objects to be boxy or diamond shaped when too many layers are added. However, with the growth method that is defined now, we can follow the signal into the noise with any shape. The appropriate quantile depends on your dataset's correlated noise properties and how cleanly it was Sky subtracted. The new @option{--detgrowmaxholesize} can also be used to specify the maximum hole size to fill as part of this growth, see the description in @ref{Detection options} for more details. This new growth process can be much more successful in detecting diffuse flux around true detections compared to dilation and give more realistic results, but it can also increase the NoiseChisel run time (depending on the given value and input size). @item @option{--cleangrowndet}: A process to further clean/remove the possibility of false detections, see the descriptions under this option in @ref{Detection options}. @end itemize @node Invoking astnoisechisel, , NoiseChisel changes after publication, NoiseChisel @subsection Invoking NoiseChisel NoiseChisel will detect and segment signal in noise producing a multi-extension labeled image, ready for input into @ref{MakeCatalog} to generate a catalog or other processing. The executable name is @file{astnoisechisel} with the following general template @example $ astnoisechisel [OPTION ...] InputImage.fits @end example @noindent One line examples: @example ## Detect signal in input.fits: $ astnoisechisel input.fits ## Detect signal assuming input has 4 channels along first dimension ## and 1 along the second. Also set the regular tile size to 100 along ## both dimensions: $ astnoisechisel --numchannels=4,1 --tilesize=100,100 input.fits @end example @cindex Gaussian @noindent If NoiseChisel is to do processing (for example you don't want to get help, or see the values to each input parameter), an input image should be provided with the recognized extensions (see @ref{Arguments}). NoiseChisel shares a large set of common operations with other Gnuastro programs, mainly regarding input/output, general processing steps, and general operating modes. To help in a unified experience between all of Gnuastro's programs, these operations have the same command-line options, see @ref{Common options} for a full list. Since the common options are thoroughly discussed there, they are no longer reviewed here. You can see all the options with a short description on the command-line with the @option{--help} option, see @ref{Getting help}. NoiseChisel's input image may contain blank elements (see @ref{Blank pixels}). Blank elements will be ignored in all steps of NoiseChisel. Hence if your dataset has bad pixels which should be masked with a mask image, please use Gnuastro's @ref{Arithmetic} program (in particular its @command{where} operator) to convert those pixels to blank pixels before running NoiseChisel. Gnuastro's Arithmetic program has bitwise operators helping you select specific kinds of bad-pixels when necessary. A convolution kernel can also be optionally given. If a value (file name) is given to @option{--kernel} on the command-line or in a configuration file (see @ref{Configuration files}), then that file will be used to convolve the image prior to thresholding. Otherwise a default kernel will be used. The default kernel is a 2D Gaussian with a FWHM of 2 pixels truncated at 5 times the FWHM. This choice of the default kernel is discussed in Section 3.1.1 of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]}. See @ref{Convolution kernel} for kernel related options. NoiseChisel defines two tessellations over the input (see @ref{Tessellation}). This enables it to deal with possible gradients in the input dataset and also significantly improve speed by processing each tile on different threads. The tessellation related options are discussed in @ref{Processing options}. In particular, NoiseChisel uses two tessellations (with everything between them identical except the tile sizes): a fine-grained one with smaller tiles (mainly used in detection) and a more larger tiled one which is used for multi-threaded processing. The common Tessellation options described in @ref{Processing options} define all parameters of both tessellations, only the large tile size for the latter tessellation is set through the @option{--largetilesize} option. To inspect the tessellations on your input dataset, run NoiseChisel with @option{--checktiles}. @cartouche @noindent @strong{Usage TIP:} Frequently use the options starting with @option{--check}. Depending on what you want to detect in the data, you can often play with the parameters/options for a better result than the default parameters. You can start with @option{--checkdetection} and @option{--checksegmentation} for the main steps. For their full list please run: @example $ astnoisechisel --help | grep check @end example @end cartouche In the sections below, NoiseChisel's options are classified into three general classes to help in easy navigation. @ref{General NoiseChisel options} mainly discusses the options relating to input and those that are shared in both detection and segmentation. Options to configure the detection are described in @ref{Detection options} and @ref{Segmentation options} we discuss how you can fine-tune the segmentation of the detections. Finally in @ref{NoiseChisel output} the format of NoiseChisel's output is discussed. The order of options here follow the same logical order that the respective action takes place within NoiseChisel (note that the output of @option{--help} is sorted alphabetically). @menu * General NoiseChisel options:: General NoiseChisel preprocessing. * Detection options:: Configure detection in NoiseChisel. * Segmentation options:: Configure segmentation in NoiseChisel. * NoiseChisel output:: NoiseChisel's output format. @end menu @node General NoiseChisel options, Detection options, Invoking astnoisechisel, Invoking astnoisechisel @subsubsection General NoiseChisel options The options discussed in this section are mainly regarding the input(s), output, and some general processing options that are shared between both detection and segmentation. Recall that you can always see the full list of Gnuastro's options with the @option{--help} option. @table @option @item -k STR @itemx --kernel=STR File name of kernel to smooth the image before applying the threshold, see @ref{Convolution kernel}. The first step of NoiseChisel is to convolve/smooth the image and use the convolved image in multiple steps during the processing. It will be used to define (and later apply) the quantile threshold (see @option{--qthresh}). The convolved image is also used to define the clumps (see Section 3.2.1 and Figure 8 of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]}). The @option{--kernel} option is not mandatory. If no kernel is provided, a 2D Gaussian profile with a FWHM of 2 pixels truncated at 5 times the FWHM is used. This choice of the default kernel is discussed in Section 3.1.1 of Akhlaghi and Ichikawa [2015]. @item --khdu=STR HDU containing the kernel in the file given to the @option{--kernel} option. @item --convolved=STR Use this file as the convolved image and don't do convolution and ignore @option{--kernel}. NoiseChisel will just check the size of the given dataset is the same as the input's size. If a wrong image (with the same size) is given to this option, the results (errors, bugs, and etc) are un-predictable. So please use this option with care and in a highly controlled environment. On such scenario is discussed below. In almost all situations, as the input gets larger, the single most CPU and time consuming step in NoiseChisel is convolution (the first step in its processing). The process of testing NoiseChisel for the best parameters in a given analysis will involve running NoiseChisel multiple times: to see the effect of each new option value. Therefore, once the kernel is finalized, re-convolving the input will greatly hinder fast testing of higher-level parameters. With this option, you can convolve the input image with your chosen kernel once before running NoiseChisel, then feed it to NoiseChisel on each test run and thus save valuable time for better/more tests. To build your desired convolution kernel, you can use @ref{MakeProfiles}. To convolve the image with a given kernel you can use @ref{Convolve}. Spatial domain convolution is mandatory. In the frequency domain, blank pixels (if present) will cover the whole image and gradients will appear on the edges, see @ref{Spatial vs. Frequency domain}. Below you can see an example of such a scenario: you want to see how variation of the growth level (through the @option{--detgrowquant} option) will affect the final result. Recall that you can ignore all the extra spaces, new lines, and `@code{\}' if you are typing in the terminal (in a shell script, remove the @code{$} signs at the start of the lines). @example ## Make the kernel to convolve with. $ astmkprof --oversample=1 --kernel=gaussian,2,5 ## Convolve the input with the given kernel. $ astconvolve input.fits --kernel=kernel.fits \ --domain=spatial --output=convolved.fits ## Run NoiseChisel with seven growth quantile values. $ for g in 60 65 70 75 80 85 90; do \ astnoisechisel input.fits --convolved=convolved.fits \ --detgrowquant=0.$g --output=$g.fits; \ done @end example @item --convolvedhdu=STR The HDU/extension containing the convolved image in the file given to @option{--convolved}. @item -w STR @itemx --widekernel=STR File name of a wider kernel to use in estimating the difference of the mode and median in a tile (this difference is used to identify the significance of signal in that tile, see @ref{Quantifying signal in a tile}). This convolved image is only used for this purpose. Once the mode is found to be sufficiently close to the median, the input convolved with the sharper kernel (@option{--kernel}) is used to identify the quantile threshold (see @option{--qthresh}). Since this convolution will significantly slow down the processing, it is optional. If no image is given, the mode and median will be found on the image that is convolved with the dataset in @option{--kernel}. @item --wkhdu=STR HDU containing the kernel file given to the @option{--widekernel} option. @item -E @itemx --skysubtracted If this option is called, it is assumed that the image has already been sky subtracted once. Knowing if the sky has already been subtracted once or not is very important in estimating the Signal to noise ratio of the detections and clumps. In short an extra @mymath{\sigma_{sky}^2} must be added in the error (noise or denominator in the Signal to noise ratio) for every flux value that is present in the calculation. This can be interpreted as the error in measuring that sky value when it was subtracted by any other program. See Section 3.3 in @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]}) for a complete explanation. @item -B FLT @itemx --minskyfrac=FLT Minimum fraction (value between 0 and 1) of sky (undetected) areas in a tile for it to be considered in measuring the following detection and segmentation properties. @itemize @item Measuring the Signal to noise ratio of false detections during the false detection removal on small tiles. @item Measuring the sky value (average of undetected pixels) on small tiles. Both before the removal of false detections and after it. @item Clump Signal to noise ratio in the sky regions of large files. @end itemize Because of the PSF and their intrinsic amorphous properties, astronomical objects (except cosmic rays) never have a clear cutoff and commonly sink into the noise very slowly. Even below the very low thresholds used by NoiseChisel. So when a large fraction of the area of one mesh is covered by detections, it is very plausible that their faint wings are present in the undetected regions (hence causing a bias in any measurement). To get an accurate measurement of the above parameters over the tessellation, tiles that harbor too many detected regions should be excluded. The used tiles are visible in the respective @option{--check} option of the given step. @item --minnumfalse=INT The minimum number of `pseudo-detections' (to identify false initial detections) or clumps (to identifying false clumps) found over the un-detected regions to identify a Signal-to-Noise ratio threshold. The Signal to noise ratio (S/N) of false pseudo-detections and clumps in each tile is found using the quantile of the S/N distribution of the psudo-detections and clumps over the undetected pixels in each mesh. If the number of S/N measurements is not large enough, the quantile will not be accurate (can have large scatter). For example if you set @option{--detquant=0.99} (or the top 1 percent), then it is best to have at least 100 S/N measurements. @item -L INT[,INT] @itemx --largetilesize=INT[,INT] The size of each tile for the tessellation with the larger tile sizes. Except for the tile size, all the other parameters for this tessellation are taken from the common options described in @ref{Processing options}. The format is identical to that of the @option{--tilesize} option that is discussed in that section. @item --onlydetection If this option is called, no segmentation will be done and the output will only have four extensions (no clumps extension, see @ref{NoiseChisel output}). The second extension of the output is not going to be objects but raw detections (a large region will be given one label): labeling is only done based on connectivity. The last two extensions of the output will be the Sky and its Standard deviation. This option can result in faster processing when only the noise properties of the image are desired for a catalog using another image's labels for example. A common case is when you want to measure colors or SEDs in several images. Let's say you have images in two colors: A and B. For simplicity also assume that they are exactly on the same position in the sky with the same pixel scale. You choose to set A as a reference, so you run the NoiseChisel fully on A. Then you run NoiseChisel on B with @option{--onlydetection} since you only need the noise properties of B (for the signal to noise column in its catalog). You can then run MakeCatalog on A normally, see @ref{MakeCatalog}. To run MakeCatalog on B, you simply set the object and clump labels images to those that NoiseChisel produced for A, see @ref{Invoking astmkcatalog}. @item --continueaftercheck Continue NoiseChisel after any of the options starting with @option{--check}. NoiseChisel involves many steps and as a result, there are many checks, allowing to inspect the status of the processing. The results of each step affect the next steps of processing, so, when you are want to check the status of the processing at one step, the time spent to complete NoiseChisel is just wasted/distracting time. To encourage easier experimentation with the option values, when you use any of the NoiseChisel options that start with @option{--check}, NoiseChisel will abort once all the desired check file(s) is (are) completed. If you call the @option{--continueaftercheck} option, you can disable this behavior and ask NoiseChisel to continue with the rest of the processing after completing the check file(s). @end table @node Detection options, Segmentation options, General NoiseChisel options, Invoking astnoisechisel @subsubsection Detection options Detection is the process of separating the pixels in the image into two groups: 1) Signal and 2) Noise. Through the parameters below, you can customize the detection process in NoiseChisel. Recall that you can always see the full list of Gnuastro's options with the @option{--help} option. @table @option @item -r FLT @itemx --mirrordist=FLT Maximum distance (as a multiple of error) to estimate the difference between the input and mirror distributions in finding the mode, see Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa 2015}, also see @ref{Quantifying signal in a tile}. @item -Q FLT @itemx --modmedqdiff=FLT The maximum acceptable distance between the mode and median, see @ref{Quantifying signal in a tile}. The quantile threshold will be found on tiles that satisfy this mode and median difference. @item -t FLT @itemx --qthresh=FLT The quantile threshold to apply to the convolved image. The detection process begins with applying a quantile threshold to each of the tiles in the small tessellation. The quantile is only calculated for tiles that don't have any significant signal within them, see @ref{Quantifying signal in a tile}. Interpolation is then used to give a value to the un-successful tiles and it is finally smoothed. @cindex Quantile @cindex Binary image @cindex Foreground pixels @cindex Background pixels The quantile value is a floating point value between 0 and 1. Assume that we have sorted the @mymath{N} data elements of a distribution (the pixels in each mesh on the convolved image). The quantile (@mymath{q}) of this distribution is the value of the element with an index of (the nearest integer to) @mymath{q\times{N}} in the sorted data set. After thresholding is complete, we will have a binary (two valued) image. The pixels above the threshold are known as foreground pixels (have a value of 1) while those which lie below the threshold are known as background (have a value of 0). @item --qthreshtilequant=FLT Only keep tiles which have a q-thresh value above the given quantile of the all successful tiles. Hence, when given a value of @code{1}, this option will be ignored. When there is more than one channel (and @option{--workoverch} is not called), quantile calculation and application will be done on each channel independently. This option is useful when a large and diffuse (almost flat within each tile) signal exists with very small regions of Sky. The flatness of the profile will cause it to successfully pass the tests of @ref{Quantifying signal in a tile}. As a result, without this option the flat and diffuse signal will be interpretted as sky. In such cases, you can see the status of the tiles with the @option{--checkqthresh} option (first image extension is enough) and select a quantile through this option to ignore the measured values in the higher-valued tiles. This option can also be useful when there are large bright objects in the image with large flat wings which can also pass the tests and give outlier values. When there is a sky gradient over the image (mainly due to post-processing issues like bad flat fielding), this option must be set to @code{1} so it is completely ignored and the sky gradient is accurately measured and subtracted. To get an estimate of the measured qthresh distribution, you can run the following commands. The first will create the qthresh check image with one value/pixel per tile (see @ref{Processing options}). Open the image in a FITS viewer and inspect it. The second command below will print the basic information about the distribution of values and the third will print the value at the 0.4 quantile. Recall that Gnuastro's Statistics program ignores blank values (in this case: tiles with significant signal), see @ref{Statistics}. @example $ astnoisechisel image.fits --checkqthresh --oneelempertile $ aststatistics image_qthresh.fits $ aststatistics image_qthresh.fits --quantile=0.4 @end example @item --smoothwidth=INT Width of flat kernel used to smooth the interpolated quantile thresholds, see @option{--qthresh} for more. @cindex NaN @item --checkqthresh Check the quantile threshold values on the mesh grid. A file suffixed with @file{_qthresh.fits} will be created showing each step. With this option, NoiseChisel will abort as soon as quantile estimation has been completed, allowing you to inspect the steps leading to the final quantile threshold, this can be disabled with @option{--continueaftercheck}. By default the output will have the same pixel size as the input, but with the @option{--oneelempertile} option, only one pixel will be used for each tile (see @ref{Processing options}). @item -e INT @itemx --erode=INT @cindex Erosion The number of erosions to apply to the binary thresholded image. Erosion is simply the process of flipping (from 1 to 0) any of the foreground pixels that neighbor a background pixel. In a 2D image, there are two kinds of neighbors, 4-connected and 8-connected neighbors. You can specify which type of neighbors should be used for erosion with the @option{--erodengb} option, see below. Erosion has the effect of shrinking the foreground pixels. To put it another way, it expands the holes. This is a founding principle in NoiseChisel: it exploits the fact that with very low thresholds, the holes in the very low surface brightness regions of an image will be smaller than regions that have no signal. Therefore by expanding those holes, we are able to separate the regions harboring signal. @item --erodengb=INT The type of neighborhood (structuring element) used in erosion, see @option{--erode} for an explanation on erosion. Only two integer values are acceptable: 4 or 8. In 4-connectivity, the neighbors of a pixel are defined as the four pixels on the top, bottom, right and left of a pixel that share an edge with it. The 8-connected neighbors on the other hand include the 4-connected neighbors along with the other 4 pixels that share a corner with this pixel. See Figure 6 (a) and (b) in Akhlaghi and Ichikawa (2015) for a demonstration. @item --noerodequant Pure erosion is going to carve off sharp and small objects completely out of the detected regions. This option can be used to avoid missing such sharp and small objects (which have significant pixels, but not over a large area). All pixels with a value larger than the significance level specified by this option will not be eroded during the erosion step above. However, they will undergo the erosion and dilation of the opening step below. Like the @option{--qthresh} option, the significance level is determined using the quantile (a value between 0 and 1). Just as a reminder, in the normal distribution, @mymath{1\sigma}, @mymath{1.5\sigma}, and @mymath{2\sigma} are approximately on the 0.84, 0.93, and 0.98 quantiles. @item -p INT @itemx --opening=INT Depth of opening to be applied to the eroded binary image. Opening is a composite operation. When opening a binary image with a depth of @mymath{n}, @mymath{n} erosions (explained in @option{--erode}) are followed by @mymath{n} dilations. Simply put, dilation is the inverse of erosion. When dilating an image any background pixel is flipped (from 0 to 1) to become a foreground pixel. Dilation has the effect of fattening the foreground. Note that in NoiseChisel, the erosion which is part of opening is independent of the initial erosion that is done on the thresholded image (explained in @option{--erode}). The structuring element for the opening can be specified with the @option{--openingngb} option. Opening has the effect of removing the thin foreground connections (mostly noise) between separate foreground `islands' (detections) thereby completely isolating them. Once opening is complete, we have @emph{initial} detections. @item --openingngb=INT The structuring element used for opening, see @option{--erodengb} for more information about a structuring element. @item -s FLT,FLT @itemx --sigmaclip=FLT,FLT The @mymath{\sigma}-clipping parameters, see @ref{Sigma clipping}. This option takes two values which are separated by a comma (@key{,}). Each value can either be written as a single number or as a fraction of two numbers (for example @code{3,1/10}). The first value to this option is the multiple of @mymath{\sigma} that will be clipped (@mymath{\alpha} in that section). The second value is the exit criteria. If it is less than 1, then it is interpreted as tolerance and if it is larger than one it is assumed to be the fixed number of iterations. Hence, in the latter case the value must be an integer. @item --checkdetsky Check the initial approximation of the sky value and its standard deviation in a FITS file ending with @file{_detsky.fits}. With this option, NoiseChisel will abort as soon as the sky value used for defining pseudo-detections is complete. This allows you to inspect the steps leading to the final quantile threshold, this behavior can be disabled with @option{--continueaftercheck}. By default the output will have the same pixel size as the input, but with the @option{--oneelempertile} option, only one pixel will be used for each tile (see @ref{Processing options}). @item -R FLT @itemx --dthresh=FLT The detection threshold: a multiple of the initial sky standard deviation added with the initial sky approximation (which you can inspect with @option{--checkdetsky}). This flux threshold is applied to the initially undetected regions on the un-convolved image. The background pixels that are completely engulfed in a 4-connected foreground region are converted to background (holes are filled) and one opening (depth of 1) is applied over both the initially detected and undetected regions. The Signal to noise ratio of the resulting `psudo-detections' are used to identify true vs. false detections. See Section 3.1.5 and Figure 7 in Akhlaghi and Ichikawa (2015) for a very complete explanation. @item -i INT @itemx --detsnminarea=INT The minimum area to calculate the Signal to noise ratio on the psudo-detections of both the initially detected and undetected regions. When the area in a psudo-detection is too small, the Signal to noise ratio measurements will not be accurate and their distribution will be heavily skewed to the positive. So it is best to ignore any psudo-detection that is smaller than this area. Use @option{--detsnhistnbins} to check if this value is reasonable or not. @item --checkdetsn Save the S/N values of the pseudo-detections and dilated detections into three files ending with @file{_detsn_sky.XXX}, @file{_detsn_det.XXX}, and @file{_detsn_dilated.XXX}. The @file{.XXX} is determined from the @option{--tableformat} option (see @ref{Input output options}, for example @file{.txt} or @file{.fits}). You can use these to inspect the S/N values and their distribution (in combination with the @option{--checkdetection} option to see where the pseudo-detections are). You can use Gnuastro's @ref{Statistics} to make a histogram of the distribution or any other analysis you would like for better understanding of the distribution (for example through a histogram). With this option, NoiseChisel will abort as soon as the tables are created. This allows you to inspect the steps leading to the final quantile threshold, this behavior (to abort NoiseChisel) can be disabled with @option{--continueaftercheck}. @item -c FLT @itemx --detquant=FLT The quantile of the Signal to noise ratio distribution of the psudo-detections in each mesh to use for filling the large mesh grid. Note that this is only calculated for the large mesh grids that satisfy the minimum fraction of undetected pixels (value of @option{--minbfrac}) and minimum number of psudo-detections (value of @option{--minnumfalse}). @item -d FLT @itemx --detgrowquant=FLT Quantile limit to ``grow'' the final detections. As discussed in the previous options, after applying the initial quantile threshold, layers of pixels are carved off the objects to identify true signal. With this step you can return those low surface brightness layers that were carved off back to the detections. To disable growth, set the value of this option to @code{1}. The process is as follows: after the true detections are found, all the non-detected pixels above this quantile will be put in a list and used to ``grow'' the true detections (seeds of the growth). Like all quantile thresholds, this threshold is defined and applied to the convolved dataset. Afterwards, the dataset is dilated once (with minimum connectivity) to connect very thin regions on the boundary: imagine building a dam at the point rivers spill into an open sea/ocean. Finally, all holes are filled. In the geography metaphor, holes can be seen as the closed (by the dams) rivers and lakes, so this process is like turning the water in all such rivers and lakes into soil. See @option{--detgrowmaxholesize} for configuring the hole filling. @item --detgrowmaxholesize=INT The maximum hole size to fill during the final expansion of the true detections as described in @option{--detgrowquant}. This is necessary when the input contains many smaller objects and can be used to avoid marking blank sky regions as detections. For example multiple galaxies can be positioned such that they surround an empty region of sky. If all the holes are filled, the Sky region in between them will be taken as a detection which is not desired. To avoid such cases, the integer given to this option must be smaller than the hole between the objects. On the other hand, if you have a very large (and extended) galaxy, the diffuse wings of the galaxy may create very large holes. In such cases, a larger value to this option will cause the whole region to be detected as part of the large galaxy and thus detect it to extremely low surface brightness limits. @item --cleangrowndet After dilation, if the signal-to-noise ratio of a detection is less than the derived pseudo-detection S/N limit, that detection will be discarded. In an ideal/clean noise, a true detection's S/N should be larger than its constituent pseudo-detections because its area is larger and it also covers more signal. However, on a false detections (especially at lower @option{--detquant} values), the increase in size can cause a decrease in S/N below that threshold. This will improve purity and not change completeness (a true detection will not be discarded). Because a true detection has flux in its vicinity and dilation will catch more of that flux and increase the S/N. So on a true detection, the final S/N cannot be less than pseudo-detections. However, in many real images bad processing creates artifacts that cannot be accurately removed by the Sky subtraction. In such cases, this option will decrease the completeness (will artificially discard true detections). So this feature is not default and should to be explicitly called when you know the noise is clean. @item --checkdetection Every step of the detection process will be added as an extension to a file with the suffix @file{_det.fits}. Going through each would just be a repeat of the explanations above and also of those in Akhlaghi and Ichikawa (2015). The extension label should be sufficient to recognize which step you are observing. Viewing all the steps can be the best guide in choosing the best set of parameters. With this option, NoiseChisel will abort as soon as a snapshot of all the detection process is saved. This behavior can be disabled with @option{--continueaftercheck}. @item --checksky Check the derivation of the final sky and its standard deviation values on the mesh grid. With this option, NoiseChisel will abort as soon as the sky value is estimated over the image (on each tile). This behavior can be disabled with @option{--continueaftercheck}. By default the output will have the same pixel size as the input, but with the @option{--oneelempertile} option, only one pixel will be used for each tile (see @ref{Processing options}). @end table @node Segmentation options, NoiseChisel output, Detection options, Invoking astnoisechisel @subsubsection Segmentation options Segmentation is the process of (possibly) breaking up a detection into multiple segments (technically called @emph{objects} and @emph{clumps} in NoiseChisel). In deep surveys segmentation becomes particularly important because we will be detecting more diffuse flux so galaxy images are going to overlap more. It is thus very important to be able separate the pixels within a detection. In NoiseChisel, segmentation is done by first finding the `true' clumps over a detection and then expanding those clumps to a certain flux limit. True clumps are found in a process very similar to the true detections explained in @ref{Detection options}, see @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]} for more information. If the connections between the grown clumps are weaker than a given threshold, the grown clumps are considered to be separate objects. @table @option @item -m INT @itemx --segsnminarea=INT The minimum area which a clump in the undetected regions should have in order to be considered in the clump Signal to noise ratio measurement. If this size is set to a small value, the Signal to noise ratio of false clumps will not be accurately found. It is recommended that this value be larger than the value to @option{--detsnminarea}. Because the clumps are found on the convolved (smoothed) image while the psudo-detections are found on the input image. You can use @option{--checkclumpsn} and @option{--checksegmentation} to see if your chosen value is reasonable or not. @item --checkclumpsn Save the S/N values of the clumps into two files ending with @file{_clumpsn_sky.XXX} and @file{_clumpsn_det.XXX}. The @file{.XXX} is determined from the @option{--tableformat} option (see @ref{Input output options}, for example @file{.txt} or @file{.fits}). You can use these to inspect the S/N values and their distribution (in combination with the @option{--checksegmentation} option to see where the clumps are). You can use Gnuastro's @ref{Statistics} to make a histogram of the distribution (ready for plotting in a text file, or a crude ASCII-art demonstration on the command-line). With this option, NoiseChisel will abort as soon as the two tables are created. This allows you to inspect the steps leading to the final S/N quantile threshold, this behavior can be disabled with @option{--continueaftercheck}. @item -g FLT @itemx --segquant=FLT The quantile of the noise clump Signal to noise ratio distribution. This value is used to identify true clumps over the detected regions. You can get the full distribution of clumps S/Ns over the undetected areas with the @option{--checkclumpsn} option and see them with @option{--checksegmentation}. @item -v @itemx --keepmaxnearriver Keep a clump whose maximum flux is 8-connected to a river pixel. By default such clumps over detections are considered to be noise and are removed irrespective of their brightness (see @ref{Flux Brightness and magnitude}). Over large profiles, that sink into the noise very slowly, noise can cause part of the profile (which was flat without noise) to become a very large and with a very high Signal to noise ratio. In such cases, the pixel with the maximum flux in the clump will be immediately touching a river pixel. @item -G FLT @itemx --gthresh=FLT Threshold (multiple of the sky standard deviation added with the sky) to stop growing true clumps. Once true clumps are found, they are set as the basis to segment the detected region. They are grown until the threshold specified by this option. @item -y INT @itemx --minriverlength=INT The minimum length of a river between two grown clumps for it to be considered in Signal to noise ratio estimations. Similar to @option{--segsnminarea} and @option{--detsnminarea}, if the length of the river is too short, the Signal to noise ratio can be noisy and unreliable. Any existing rivers shorter than this length will be considered as non-existent, independent of their Signal to noise ratio. Since the clumps are grown on the input image, this value should best be similar to the value of @option{--detsnminarea}. Recall that the clumps were defined on the convolved image so @option{--segsnminarea} was larger than @option{--detsnminarea}. @item -O FLT @itemx --objbordersn=FLT The maximum Signal to noise ratio of the rivers between two grown clumps in order to consider them as separate `objects'. If the Signal to noise ratio of the river between two grown clumps is larger than this value, they are defined to be part of one `object'. Note that the physical reality of these `objects' can never be established with one image, or even multiple images from one broad-band filter. Any method we devise to define `object's over a detected region is ultimately subjective. Two very distant galaxies or satellites in one halo might lie in the same line of sight and be detected as clumps on one detection. On the other hand, the connection (through a spiral arm or tidal tail for example) between two parts of one galaxy might have such a low surface brightness that they are broken up into multiple detections or objects. In fact if you have noticed, exactly for this purpose, this is the only Signal to noise ratio that the user gives into NoiseChisel. The `true' detections and clumps can be objectively identified from the noise characteristics of the image, so you don't have to give any hand input Signal to noise ratio. @item --grownclumps In the output (see @ref{NoiseChisel output}) store the grown clumps (or full detected region if only one clump was present in that detection). By default the original clumps are stored as the third extension of the output, if this option is called, it is replaced with the grown clump labels. @item --checksegmentation A file with the suffix @file{_seg.fits} will be created. This file keeps all the relevant steps in finding true clumps and segmenting the detections into multiple objects in various extensions. Having read the paper or the steps above. Examining this file can be an excellent guide in choosing the best set of parameters. Note that calling this function will significantly slow NoiseChisel. In verbose mode (without the @option{--quiet} option, see @ref{Operating mode options}) the important steps (along with their extension names) will also be reported. With this option, NoiseChisel will abort as soon as the two tables are created. This behavior can be disabled with @option{--continueaftercheck}. @end table @node NoiseChisel output, , Segmentation options, Invoking astnoisechisel @subsubsection NoiseChisel output The default name and directory of the outputs are explained in @ref{Automatic output}. NoiseChisel's default output (when none of the options starting with @option{--check} or the @option{--output} option are called) is one file ending with @file{_labeled.fits}. This file has the extensions listed below: @enumerate @item A copy of the input image, a copy is placed here for the following reasons: @itemize @item By flipping through the extensions, a user can check how accurate the detection and segmentation process was. @item All the inputs to MakeCatalog (see @ref{MakeCatalog}) are included in this one file which makes the running of MakeCatalog after NoiseChisel very easy. @end itemize @item The object/detection labels. Each pixel in the input image is given a label in this extension, the labels start from one. If the @option{--onlydetection} option is given, each large connected part of the image has one label. Without that option, this extension is going to show the labels of the objects that are found after segmentation. The total number of labels is stored as the value to the @code{NOBJS}/@code{NDETS} keyword in the header of this extension. This number is also printed in verbose mode. @item The clump labels when @option{--onlydetection} is not called. All the pixels in the input image that belong to a true clump are given a positive label in this extension. The detected regions that were not a clump are given a negative value to clearly identify the sky noise from the diffuse detections. The total number of clumps in this image is stored in the @code{NCLUMPS} keyword of this extension and printed in verbose output. If the @option{--grownclumps} option is called, or a value of @code{1} is given to it in any of the configuration files, then instead of the original clump regions, the grown clumps will be stored in this extension. Note that if there is only one clump (or no clumps) over a detected region, then the whole detected region is given a label of 1. @item The final sky value on each pixel. See @ref{Sky value} for a complete explanation. @item Similar to the previous mesh but for the standard deviation on each pixel. @end enumerate To inspect NoiseChisel's output, you can configure SAO DS9 in your Graphic User Interface (GUI) to open NoiseChisel's output as a multi-extension data cube. This will allow you to flip through the different extensions and visually inspect the results. This process has been described for the GNOME GUI (most common GUI in GNU/Linux operating systems) in @ref{Viewing multiextension FITS images}. @node MakeCatalog, Match, NoiseChisel, Data analysis @section MakeCatalog At the lowest level, a dataset (for example an image) is just a collection of values, placed after each other in any number of dimensions (for example an image is a 2D dataset). Each data-element (pixel) just has two properties: its position (relative to the rest) and its value. The entire input dataset (a large image for example) is rarely treated as a singular entity for higher-level analysis@footnote{In low-level reduction/preparation of a dataset, you do in fact treat a whole image as a single entity. You can derive the over-all properties of all the pixels in a dataset with Gnuastro's Statistics program (see @ref{Statistics})}. You want to know the properties of the scientifically interesting targets that are embedded in it. For example the magnitudes, positions and elliptical properties of the galaxies that are in the image. MakeCatalog is Gnuastro's program to derive higher-level information for @emph{pre-defined} regions of a dataset. The role of MakeCatalog in a scientific analysis and the benefits of this model of data-analysis (were detection/identification is separated from measurement) is discussed in @url{https://arxiv.org/abs/1611.06387v1, Akhlaghi [2016]}. We strongly recommend reading this short paper for a better understanding of this methodology and use MakeCatalog most effectively. However, that paper cannot undergo any more change, so this manual is the definitive guide. As discussed above, you have to define the regions of a dataset that you are interested in @emph{before} running MakeCatalog. MakeProfiles currently uses labeled dataset(s) for this job. A labeled dataset for a given input dataset has the size/dimensions as the input, but its pixels have an integer type (see @ref{Numeric data types})@footnote{If the program you used to generate the labeled image only outputs floating point types, but you know it only has integer valued pixels that are stored in a floating point container, you can use Gnuastro's Arithmetic program (see @ref{Arithmetic}) to change the numerical data type of the image (@file{flabel.fits}) to an integer type image (@file{label.fits}) with a command like below:@*@command{$ astarithmetic flabel.fits int32 --output=label.fits}}: all pixels with the same label (integers larger and equal to one) are used to generate the requested output columns of MakeCatalog for the row of their labeled value. For example, the flux weighted average position of all the pixels with a label of 42 will be considered as the central position@footnote{See @ref{Measuring elliptical parameters} for a discussion on this and the derivation of positional parameters.} of the 42nd row of the output catalog. Pixels with labels equal to or smaller than zero will be ignored by MakeCatalog. In other words, the number of rows of the output catalog will be determined from the labeled image. The labeled image maybe created with any tool@footnote{For example, you can even use a graphic user interface image editing tool like the GNU Image Manipulation Program (or GIMP) and use Gnuastro's ConvertType to convert it to a FITS file.}. Within Gnuastro you can use these two solutions depending on a-priori/parametric knowledge of the targets you want to study: @itemize @cindex Aperture photometry @cindex Photometry, aperture @item When you already know the positions and parametric (for example circular or elliptical) properties of the targets, you can use @ref{MakeProfiles} to generate a labeled image from another catalog. This is also known as aperture photometry (the apertures are defined a-priori). @item When the shape of your targets cannot be parameterized accurately (for example galaxies), or if you don't know the number/shape of the targets in the image, you can use Gnuastro's NoiseChisel program to detect and segment (make labeled images of) the @emph{objects} and @emph{clumps} in the input image, see @ref{NoiseChisel}. @end itemize @menu * Detection and catalog production:: Discussing why/how to treat these separately * Quantifying measurement limits:: For comparing different catalogs. * Measuring elliptical parameters:: Estimating elliptical parameters. * Adding new columns to MakeCatalog:: How to add new columns. * Invoking astmkcatalog:: Options and arguments to MakeCatalog. @end menu @node Detection and catalog production, Quantifying measurement limits, MakeCatalog, MakeCatalog @subsection Detection and catalog production As discussed above (@ref{MakeCatalog}), NoiseChisel (Gnuastro's signal detection tool, see @ref{NoiseChisel}) does not produce any catalog of the detected objects. However, most other common tools in astronomical data-analysis (for example SExtractor@footnote{@url{https://www.astromatic.net/software/sextractor}}) merge the two processes into one. Gnuastro's modularized methodology is therefore new to many experienced astronomers and deserves a short review here. Further discussion on the benefits of this methodology can be seen in @url{https://arxiv.org/abs/1611.06387v1, Akhlaghi [2016]}. To simplify catalog production from a raw input image in Gnuastro, NoiseChisel's output (see @ref{NoiseChisel output}) can be directly fed into MakeCatalog. This is good when no further customization is necessary and you want a fast/simple. But the modular approach taken by Gnuastro has many benefits that will become more apparent as you get more experienced in astronomical data analysis and want to be more creative in using your valuable data for the exciting scientific project you are working on. In short the reasons for this modularity can be classified as below: @itemize @item Complexity of a monolith: Adding in a catalog functionality to the detector program will add several more steps (and many more options) to its processing that can equally well be done outside of it. This makes following what the program does harder for the users and developers, it can also potentially add many bugs. As an example, if the parameter you want to measure over one profile is not provided by the developers of MakeCatalog. You can simply open this tiny little program and add your desired calculation easily. This process is discussed in @ref{Adding new columns to MakeCatalog}. However, if making a catalog was part of NoiseChisel, it would require a lot of energy to understand all the steps and internal structures of that large program (the most complex in Gnuastro) in order to add desired parameter in a catalog. @item Simplicity/robustness of independent, modular tools: making a catalog is a logically separate process from labeling (detection and segmentation). A user might want to do certain operations on the labeled regions before creating a catalog for them. Another user might want the properties of the same pixels/objects in another image (another filter for example) to measure the colors or SED fittings. Here is an example of doing both: suppose you have images in various broad band filters at various resolutions and orientations. The image of one color will thus not lie exactly on another or even be in the same scale. However, it is imperative that the same pixels be used in measuring the colors of galaxies. To solve the problem, NoiseChisel can be run on the reference image to generate the labeled image. After wards, the labeled image can be warped into the grid of the other color (using @ref{Warp}). MakeCatalog will then generate the same catalog for both colors (with the different labeled images). It is currently customary to warp the images to the same pixel grid, however, modification of the scientific dataset is very harmful for the data and creates correlated noise. It is much more accurate to do the transformations on the labeled image. @end itemize @node Quantifying measurement limits, Measuring elliptical parameters, Detection and catalog production, MakeCatalog @subsection Quantifying measurement limits @cindex Depth @cindex Clump magnitude limit @cindex Object magnitude limit @cindex Limit, object/clump magnitude @cindex Magnitude, object/clump detection limit No measurement on a real dataset can be perfect: you can only reach a certain level/limit of accuracy. Therefore, a meaningful (scientific) analysis requires an understanding of these limits for the dataset and your analysis tools: different datasets (images in the case of MakeCatalog) have different noise properties and different detection methods (one method/algorith/software that is run with a different set of parameters is considered as a different detection method) will have different abilities to detect or measure certain kinds of signal (astronomical objects) and their properties in an image. Hence, quantifying the detection and measurement limitations with a particular dataset and analysis tool is the most crucial/critical aspect of any high-level analysis. In this section we discuss some of the most general limits that are very important in any astronomical data analysis and how MakeCatalog makes it easy to find them. Depending on the higher-level analysis, there are more tests that must be done, but these are usually necessary in any case. In astronomy, it is common to use the magnitude (a unit-less scale) and physical units, see @ref{Flux Brightness and magnitude}. Therefore all the measurements discussed here are defined in units of magnitudes. @table @asis @item Surface brightness limit (of whole dataset) @cindex Surface brightness As we make more observations on one region of the sky, and add the observations into one dataset, we are able to decrease the standard deviation of the noise in each pixel@footnote{This is true for any noisy data, not just astronomical images.}. Qualitatively, this decrease manifests its self by making fainter (per pixel) parts of the objects in the image more visible. Technically, this is known as surface brightness. Quantitatively, it increases the Signal to noise ratio, since the signal increases faster than noise with more data. It is very important to have in mind that here, noise is defined per pixel (or in the units of our data measurement), not per object. You can think of the noise as muddy water that is completely covering a flat ground@footnote{The ground is the sky value in this analogy, see @ref{Sky value}. Note that this analogy only holds for a flat sky value across the surface of the image or ground.} with some regions higher than the others@footnote{The peaks are the brightest parts of astronomical objects in this analogy.} in it. In this analogy, height (from the ground) is @emph{surface brightness}. Let's assume that in your first observation the muddy water has just been stirred and you can't see anything through it. As you wait and make more observations, the mud settles down and the @emph{depth} of the transparent water increases, making the summits of hills visible. As the depth of clear water increases, the parts of the hills with lower heights (less parts with lower surface brightness) can be seen more clearly. @cindex Data's depth The outputs of NoiseChisel include the Sky standard deviation (@mymath{\sigma}) on every group of pixels (a mesh) that were calculated from the undetected pixels in that mesh, see @ref{Tessellation} and @ref{NoiseChisel output}. Let's take @mymath{\sigma_m} as the median @mymath{\sigma} over the successful meshes in the image (prior to interpolation or smoothing). On different instruments pixels have different physical sizes (for example in micro-meters, or spatial angle over the sky), nevertheless, a pixel is our unit of data collection. In other words, while quantifying the noise, the physical or projected size of the pixels is irrelevant. We thus define the Surface brightness limit or @emph{depth}, in units of magnitude/pixel, of a data-set, with zeropoint magnitude @mymath{z}, with the @mymath{n}th multiple of @mymath{\sigma_m} as (see @ref{Flux Brightness and magnitude}): @dispmath{SB_{\rm Pixel}=-2.5\times\log_{10}{(n\sigma_m)}+z} @cindex XDF @cindex CANDELS As an example, the XDF survey covers part of the sky that the Hubble space telescope has observed the most (for 85 orbits) and is consequently very small (@mymath{\sim4} arcmin@mymath{^2}). On the other hand, the CANDELS survey, is one of the widest multi-color surveys covering several fields (about 720 arcmin@mymath{^2}) but its deepest fields have only 9 orbits observation. The depth of the XDF and CANDELS-deep surveys in the near infrared WFC3/F160W filter are respectively 34.40 and 32.45 magnitudes/pixel. In a single orbit image, this same field has a depth of 31.32. Recall that a larger magnitude corresponds to less brightness. The low-level magnitude/pixel measurement above is only useful when all the datasets you want to use belong to one instrument (telescope and camera). However, you will often find yourself using datasets from various instruments with different pixel scales (projected pixel sizes). If we know the pixel scale, we can obtain a more easily comparable surface brightness limit in units of: magnitude/arcsec@mymath{^2}. Let's assume that the dataset has a zeropoint value of @mymath{z}, and every pixel is @mymath{p} arcsec@mymath{^2} (so @mymath{A/p} is the number of pixels that cover an area of @mymath{A} arcsec@mymath{^2}). If the @mymath{n}th multiple of @mymath{\sigma_m} is desired, then the surface brightness (in units of magnitudes per A arcsec@mymath{^2}) is@footnote{If we have @mymath{N} datasets, each with noise @mymath{\sigma}, the noise of a combined dataset will increase as @mymath{\sqrt{N}\sigma}.}: @dispmath{SB_{\rm Projected}=-2.5\times\log_{10}{\left(n\sigma_m\sqrt{A\over p}\right)+z}} Note that this is an extrapolation of the actually measured value of @mymath{\sigma_m} (which was per pixel). So it should be used with extreme care (for example the dataset must have an approximately flat depth). For each detection over the dataset, you can estimate an upper-limit magnitude which actually uses the detection's area/footprint. It doesn't extrapolate and even accounts for correlated noise features. Therefore, the upper-limit magnitude is a much better measure of your dataset's surface brightness limit for each particular object. MakeCatalog will calculate the input dataset's @mymath{SB_{\rm Pixel}} and @mymath{SB_{\rm Projected}} and write them as comments/meta-data in the output catalog(s). Just note that @mymath{SB_{\rm Projected}} is only calculated if the input has World Coordinate System (WCS). @item Completeness limit (of each detection) @cindex Completeness As the surface brightness of the objects decreases, the ability to detect them will also decrease. An important statistic is thus the fraction of objects of similar morphology and brightness that will be identified with our detection algorithm/parameters in the given image. This fraction is known as completeness. For brighter objects, completeness is 1: all bright objects that might exist over the image will be detected. However, as we go to lower surface brightness objects, we fail to detect some and gradually we are not able to detect anything any more. For a given profile, the magnitude where the completeness drops below a certain level usually above @mymath{90\%} is known as the completeness limit. @cindex Purity @cindex False detections @cindex Detections false Another important parameter in measuring completeness is purity: the fraction of true detections to all true detections. In effect purity is the measure of contamination by false detections: the higher the purity, the lower the contamination. Completeness and purity are anti-correlated: if we can allow a large number of false detections (that we might be able to remove by other means), we can significantly increase the completeness limit. One traditional way to measure the completeness and purity of a given sample is by embedding mock profiles in regions of the image with no detection. However in such a study we must be really careful to choose model profiles as similar to the target of interest as possible. @item Magnitude measurement error (of each detection) Any measurement has an error and this includes the derived magnitude for an object. Note that this value is only meaningful when the object's magnitude is brighter than the upper-limit magnitude (see the next items in this list). As discussed in @ref{Flux Brightness and magnitude}, the magnitude (@mymath{M}) of an object with brightness @mymath{B} and Zeropoint magnitude @mymath{z} can be written as: @dispmath{M=-2.5\log_{10}(B)+z} @noindent Calculating the derivative with respect to @mymath{B}, we get: @dispmath{{dM\over dB} = {-2.5\over {B\times ln(10)}}} @noindent From the Tailor series (@mymath{\Delta{M}=dM/dB\times\Delta{B}}), we can write: @dispmath{\Delta{M} = \left|{-2.5\over ln(10)}\right|\times{\Delta{B}\over{B}}} @noindent But, @mymath{\Delta{B}/B} is just the inverse of the Signal-to-noise ratio (@mymath{S/N}), so we can write the error in magnitude in terms of the signal-to-noise ratio: @dispmath{ \Delta{M} = {2.5\over{S/N\times ln(10)}} } MakeCatalog uses this relation to estimate the magnitude errors. The signal-to-noise ratio is calculated in different ways for clumps and objects (see @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]}), but this single equation can be used to estimate the measured magnitude error afterwards for any type of target. @item Upper limit magnitude (of each detection) Due to the noisy nature of data, it is possible to get arbitrarily low values for a faint object's brightness (or arbitrarily high magnitudes). Given the scatter caused by the noise, such small values are meaningless: another similar depth observation will give a radically different value. This problem is most common when you use one image/filter to generate target labels (which specify which pixels belong to which object, see @ref{NoiseChisel output} and @ref{MakeCatalog}) and another image/filter to generate a catalog for measuring colors. The object might not be visible in the filter used for the latter image, or the image @emph{depth} (see above) might be much shallower. So you will get unreasonably faint magnitudes. For example when the depth of the image is 32 magnitudes, a measurement that gives a magnitude of 36 for a @mymath{\sim100} pixel object is clearly unreliable. In another similar depth image, we might measure a magnitude of 30 for it, and yet another might give 33. Furthermore, due to the noise scatter so close to the depth of the data-set, the total brightness might actually get measured as a negative value, so no magnitude can be defined (recall that a magnitude is a base-10 logarithm). @cindex Upper limit magnitude @cindex Magnitude, upper limit Using such unreliable measurements will directly affect our analysis, so we must not use them. However, all is not lost! Given our limited depth, there is one thing we can deduce about the object's magnitude: we can say that if something actually exists here (possibly buried deep under the noise), it must have a magnitude that is fainter than an @emph{upper limit magnitude}. To find this upper limit magnitude, we place the object's footprint (segmentation map) over random parts of the image where there are no detections, so we only have pure (possibly correlated) noise and undetected objects. Doing this a large number of times will give us a distribution of brightness values. The standard deviation (@mymath{\sigma}) of that distribution can be used to quantify the upper limit magnitude. @cindex Correlated noise Traditionally, faint/small object photometry was done using fixed circular apertures (for example with a diameter of @mymath{N} arc-seconds). In this way, the upper limit was like the depth discussed above: one value for the whole image. But with the much more advanced hardware and software of today, we can make customized segmentation maps for each object. The number of pixels (are of the object) used directly affects the final distribution and thus magnitude. Also the image correlated noise might actually create certain patters, so the shape of the object can also affect the result. So in MakeCatalog, the upper limit magnitude is found for each object in the image separately. Not one value for the whole image. @end table @node Measuring elliptical parameters, Adding new columns to MakeCatalog, Quantifying measurement limits, MakeCatalog @subsection Measuring elliptical parameters The shape or morphology of a target is one of the most commonly desired parameters of a target. Here, we will review the derivation of the most basic/simple morphological parameters: the elliptical parameters for a set of labeled pixels. The elliptical parameters are: the (semi-)major axis, the (semi-)minor axis and the position angle along with the central position of the profile. The derivations below follow the SExtractor manual derivations with some added explanations for easier reading. @cindex Moments Let's begin with one dimension for simplicity: Assume we have a set of @mymath{N} values @mymath{B_i} (keeping the spatial distribution of brightness for example), each at position @mymath{x_i}. The simplest parameter we can define is the geometric center of the object (@mymath{x_g}) (ignoring the brightness values): @mymath{x_g=(\sum_ix_i)/N}. @emph{Moments} are defined to incorporate both the value (brightness) and position of the data. The first moment can be written as: @dispmath{\overline{x}={\sum_iB_ix_i \over \sum_iB_i}} @cindex Variance @cindex Second moment @noindent This is essentially the weighted (by @mymath{B_i}) mean position. The geometric center (@mymath{x_g}, defined above) is a special case of this with all @mymath{B_i=1}. The second moment is essentially the variance of the distribution: @dispmath{\overline{x^2}\equiv{\sum_iB_i(x_i-\overline{x})^2 \over \sum_iB_i} = {\sum_iB_ix_i^2 \over \sum_iB_i} - 2\overline{x}{\sum_iB_ix_i\over\sum_iB_i} + \overline{x}^2 ={\sum_iB_ix_i^2 \over \sum_iB_i} - \overline{x}^2} @cindex Standard deviation @noindent The last step was done from the definition of @mymath{\overline{x}}. Hence, the square root of @mymath{\overline{x^2}} is the spatial standard deviation (along the one-dimension) of this particular brightness distribution (@mymath{B_i}). Crudely (or qualitatively), you can think of its square root as the distance (from @mymath{\overline{x}}) which contains a specific amount of the flux (depending on the @mymath{B_i} distribution). Similar to the first moment, the geometric second moment can be found by setting all @mymath{B_i=1}. So while the first moment quantified the position of the brightness distribution, the second moment quantifies how that brightness is dispersed about the first moment. In other words, it quantifies how ``sharp'' the object's image is. @cindex Floating point error Before continuing to two dimensions and the derivation of the elliptical parameters, let's pause for an important implementation technicality. You can ignore this paragraph and the next two if you don't want to implement these concepts. The basic definition (first definition of @mymath{\overline{x^2}} above) can be used without any major problem. However, using this fraction requires two runs over the data: one run to find @mymath{\overline{x}} and another run to find @mymath{\overline{x^2}} from @mymath{\overline{x}}, this can be slow. The advantage of the last fraction above, is that we can estimate both the first and second moments in one run (since the @mymath{-\overline{x}^2} term can easily be added later). The logarithmic nature of floating point number digitization creates a complication however: suppose the object is located between pixels 10000 and 10020. Hence the target's pixels are only distributed over 20 pixels (with a standard deviation @mymath{<20}), while the mean has a value of @mymath{\sim10000}. The @mymath{\sum_iB_i^2x_i^2} will go to very very large values while the individual pixel differences will be orders of magnitude smaller. This will lower the accuracy of our calculation due to the limited accuracy of floating point operations. The variance only depends on the distance of each point from the mean, so we can shift all position by a constant/arbitrary @mymath{K} which is much closer to the mean: @mymath{\overline{x-K}=\overline{x}-K}. Hence we can calculate the second order moment using: @dispmath{ \overline{x^2}={\sum_iB_i(x_i-K)^2 \over \sum_iB_i} - (\overline{x}-K)^2 } @noindent The closer @mymath{K} is to @mymath{\overline{x}}, the better (the sums of squares will involve smaller numbers), as long as @mymath{K} is within the object limits (in the example above: @mymath{10000\leq{K}\leq10020}), the floating point error induced in our calculation will be negligible. For the most simplest implementation, MakeCatalog takes @mymath{K} to be the smallest position of the object in each dimension. Since @mymath{K} is arbitrary and an implementation/technical detail, we will ignore it for the remainder of this discussion. In two dimensions, the mean and variances can be written as: @dispmath{\overline{x}={\sum_iB_ix_i\over B_i}, \quad \overline{x^2}={\sum_iB_ix_i^2 \over \sum_iB_i} - \overline{x}^2} @dispmath{\overline{y}={\sum_iB_iy_i\over B_i}, \quad \overline{y^2}={\sum_iB_iy_i^2 \over \sum_iB_i} - \overline{y}^2} @dispmath{\quad\quad\quad\quad\quad\quad\quad\quad\quad \overline{xy}={\sum_iB_ix_iy_i \over \sum_iB_i} - \overline{x}\times\overline{y}} If an elliptical profile's major axis exactly lies along the @mymath{x} axis, then @mymath{\overline{x^2}} will be directly proportional with the profile's major axis, @mymath{\overline{y^2}} with its minor axis and @mymath{\overline{xy}=0}. However, in reality we are not that lucky and (assuming galaxies can be parameterized as an ellipse) the major axis of galaxies can be in any direction on the image (in fact this is one of the core principles behind weak-lensing by shear estimation). So the purpose of the remainder of this section is to define a strategy to measure the position angle and axis ratio of some randomly positioned ellipses in an image, using the raw second moments that we have calculated above in our image coordinates. Let's assume we have rotated the galaxy by @mymath{\theta}, the new second order moments are: @dispmath{\overline{x_\theta^2} = \overline{x^2}\cos^2\theta + \overline{y^2}\sin^2\theta - 2\overline{xy}\cos\theta\sin\theta } @dispmath{\overline{y_\theta^2} = \overline{x^2}\sin^2\theta + \overline{y^2}\cos^2\theta + 2\overline{xy}\cos\theta\sin\theta} @dispmath{\overline{xy_\theta} = \overline{x^2}\cos\theta\sin\theta - \overline{y^2}\cos\theta\sin\theta + \overline{xy}(\cos^2\theta-\sin^2\theta)} @noindent The best @mymath{\theta} (@mymath{\theta_0}, where major axis lies along the @mymath{x_\theta} axis) can be found by: @dispmath{\left.{\partial \overline{x_\theta^2} \over \partial \theta}\right|_{\theta_0}=0} Taking the derivative, we get: @dispmath{2\cos\theta_0\sin\theta_0(\overline{y^2}-\overline{x^2}) + 2(\cos^2\theta_0-\sin^2\theta_0)\overline{xy}=0} When @mymath{\overline{x^2}\neq\overline{y^2}}, we can write: @dispmath{\tan2\theta_0 = 2{\overline{xy} \over \overline{x^2}-\overline{y^2}}.} @cindex Position angle @noindent MakeCatalog uses the standard C math library's @code{atan2} function to estimate @mymath{\theta_0}, which we define as the position angle of the ellipse. To recall, this is the angle of the major axis of the ellipse with the @mymath{x} axis. By definition, when the elliptical profile is rotated by @mymath{\theta_0}, then @mymath{\overline{xy_{\theta_0}}=0}, @mymath{\overline{x_{\theta_0}^2}} will be the extent of the maximum variance and @mymath{\overline{y_{\theta_0}^2}} the extent of the minimum variance (which are perpendicular for an ellipse). Replacing @mymath{\theta_0} in the equations above for @mymath{\overline{x_\theta}} and @mymath{\overline{y_\theta}}, we can get the semi-major (@mymath{A}) and semi-minor (@mymath{B}) lengths: @dispmath{A^2\equiv\overline{x_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} + \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}} @dispmath{B^2\equiv\overline{y_{\theta_0}^2}= {\overline{x^2} + \overline{y^2} \over 2} - \sqrt{\left({\overline{x^2}-\overline{y^2} \over 2}\right)^2 + \overline{xy}^2}} As a summary, it is important to remember that the units of @mymath{A} and @mymath{B} are in pixels (the standard deviation of a positional distribution) and that they represent the spatial light distribution of the object in both image dimensions (rotated by @mymath{\theta_0}). When the object cannot be represented as an ellipse, this interpretation breaks down: @mymath{\overline{xy_{\theta_0}}\neq0} and @mymath{\overline{y_{\theta_0}^2}} will not be the direction of minimum variance. @node Adding new columns to MakeCatalog, Invoking astmkcatalog, Measuring elliptical parameters, MakeCatalog @subsection Adding new columns to MakeCatalog MakeCatalog is designed to allow easy addition of different measurements over a labeled image (see @url{https://arxiv.org/abs/1611.06387v1, Akhlaghi [2016]}). A check-list style description of necessary steps to do that is described in this section. The common development characteristics of MakeCatalog and other Gnuastro programs is explained in @ref{Developing}. We strongly encourage you to have a look at that chapter to greatly simplify your navigation in the code. After adding and testing your column, you are most welcome (and encouraged) to share it with us so we can add to the next release of Gnuastro for everyone else to also benefit from your efforts. MakeCatalog will first pass over each label's pixels two times and do necessary raw/internal calculations. Once the passes are done, it will use the raw information for filling the final catalog's columns. In the first pass it will gather mainly object information and in the second run, it will mainly focus on the clumps, or any other measurement that needs an output from the first pass. These two passes are designed to be raw summations: no extra processing. This will allow parallel processing and simplicity/clarity. So if your new calculation, needs new raw information from the pixels, then you will need to also modify the respective @code{mkcatalog_first_pass} and @code{mkcatalog_second_pass} functions (both in @file{bin/mkcatalog/mkcatalog.c}) and define new raw table columns in @file{main.h} (hopefully the comments in the code are clear enough). In all these different places, the final columns are sorted in the same order (same order as @ref{Invoking astmkcatalog}). This allows a particular column/option to be easily found in all steps. Therefore in adding your new option, be sure to keep it in the same relative place in the list in all the separate places (it doesn't necessarily have to be in the end), and near conceptually similar options. @table @file @item main.h The @code{objectcols} and @code{clumpcols} enumerated variables (@code{enum}) define the raw/internal calculation columns. If your new column requires new raw calculations, add a row to the respective list. If your calculation requires any other settings parameters, you should add a variable to the @code{mkcatalogparams} structure. @item ui.h The @code{option_keys_enum} associates a unique value for each option to MakeProfiles. The options that have a short option version, the single character short comment is used for the value. Those that don't have a short option version, get a large integer automatically. You should add a variable here to identify your desired column. @cindex GNU C library @item args.h This file specifies all the parameters for the GNU C library, Argp structure that is in charge of reading the user's options. To define your new column, just copy an existing set of parameters and change the first, second and 5th values (the only ones that differ between all the columns), you should use the macro you defined in @file{ui.h} here. @item ui.c If your column includes any particular settings (you added a variable to the @code{mkcatalogparams} structure in @file{main.h}), you should do the sanity checks and preparations for it here. Otherwise, you can ignore this file. @item columns.c This file will contain the main definition and high-level calculation of your new column through the @code{columns_define_alloc} and @code{columns_fill} functions. In the first, you specify the basic information about the column: its name, units, comments, type (see @ref{Numeric data types}) and how it should be printed if the output is a text file. You should also specify the raw/internal columns that are necessary for this column here as the many existing examples show. Through the types for objects and rows, you can specify if this column is only for clumps, objects or both. The second main function (@code{columns_fill}) writes the final value into the appropriate column for each object and clump. As you can see in the many existing examples, you can define your processing on the raw/internal calculations here and save them in the output. @item mkcatalog.c As described before, this file contains the two main MakeCatalog work-horses: @code{mkcatalog_first_pass} and @code{mkcatalog_second_pass}, their names are descriptive enough and their internals are also clear and heavily commented. @end table @node Invoking astmkcatalog, , Adding new columns to MakeCatalog, MakeCatalog @subsection Invoking MakeCatalog MakeCatalog will make a catalog from an input image and at least on labeled image. The executable name is @file{astmkcatalog} with the following general template @example $ astmkcatalog [OPTION ...] InputImage.fits @end example @noindent One line examples: @example ## Create catalog with RA, Dec, Magnitude and Magnitude error, ## `input.fits' is NoiseChisel's output: $ astmkcatalog --ra --dec --magnitude --magnitudeerr input.fits ## Same catalog as above (using short options): $ asmkcatalog -rdmG input.fits ## Write the catalog to a FITS table: $ astmkcatalog -mpQ --output=cat.fits input_labeled.fits ## Read the columns to create from `columns.conf': $ astmkcatalog --config=columns.conf input_labeled.fits ## Use different images for the objects and clumps inputs: $ astmkcatalog --objectsfile=K_labeled.fits --objectshdu=1 \ --clumpsfile=K_labeled.fits --clumpshdu=2 i_band.fits @end example @cindex Gaussian @noindent If MakeCatalog is to do processing, an input image should be provided with the recognized extensions as input data, see @ref{Arguments}. The options described in this section are those that are only particular to MakeProfiles. For operations that MakeProfiles shares with other programs (mainly involving input/output or general processing steps), see @ref{Common options}. Also see @ref{Common program behavior} for some general characteristics of all Gnuastro programs including MakeCatalog. MakeCatalog needs 4 (or 5) images as input. These images can be separate extensions in one file (NoiseChisel's default output), or each can have its own file and its own extension. See @ref{NoiseChisel output} for the list. The clump labels image is not mandatory (when no clump catalog is required, for example in aperture photometry). When inspecting the object labels image, MakeProfiles will look for a @code{WCLUMPS} (short for with-clumps) header keyword. If that keyword is present and has a value of @code{yes}, @code{1}, or @code{y} (case insensitive) then a clump image must also be provided and a clump catalog will be made. When @code{WCLUMPS} isn't present or has any other value, only an object catalog will be created and all clump related options/columns will be ignored. @cindex Photometry, aperture @cindex Aperture photometry For example, if you only need an object catalog from NoiseChisel's output, you can use Gnuastro's Fits program (see @ref{Fits}) to modify or remove the @code{WCLUMPS} keyword in the objects HDU, then run MakeCatalog on it. Another example can be aperture photometry: let's assume you have made your labeled image (defining the apertures) with MakeProfiles. Clumps are not defined in this context, so besides the input and labeled image, you only need NoiseChisel's Sky and Sky standard deviation images (run NoiseChisel with the @option{--onlydetection} option). Since MakeProfile's output doesn't contain the @code{WCLUMPS} keyword, you just have to specify your labeled image with the @option{--objectsfile} option and also set its HDU. Note that labeled images have to be an integer type. Therefore, if you are using MakeProfiles to define the apertures/labels, you can use its @option{--type=int32} for example, see @ref{Input output options} and @ref{Numeric data types}. When a clump catalog is also desired, two catalogs will be made: one for the objects (suffixed with @file{_o.txt} or @file{_o.fits}) and another for the clumps (suffixed with @file{_c.txt} or @file{_c.fits}). Therefore if any value is given to the @option{--output} option, MakeCatalogs will replace these two suffixes with any existing suffix in the given value. If no output value is given, MakeCatalog will use the input name, see @ref{Automatic output}. The format of the output table is specified with the @option{--tableformat} option, see @ref{Input output options}. When MakeCatalog is run on multiple threads, the clumps catalog rows will not be sorted by object since each object is processed independently by one thread and threaded applications are asynchronous. The clumps in each object will be sorted based on their labels, but you will find lower-index objects come after higher-index ones (especially if they have more clumps and thus take more time). If the order is very important for you, you can run the following command to sort the rows by object ID (and clump ID with each object): @example $ awk '!/^#/' out_c.txt | sort -g -k1,1 -k2,2 @end example @menu * MakeCatalog input files:: Specifying the different input files. * MakeCatalog general settings:: Options for general column settings. * Upper-limit magnitude settings:: Necessary to define upper-limit magnitudes. * MakeCatalog output columns:: How to specify the columns in the output. @end menu @node MakeCatalog input files, MakeCatalog general settings, Invoking astmkcatalog, Invoking astmkcatalog @subsubsection MakeCatalog input files MakeCatalog needs multiple images as input: a values image, one (or two) labeled images and Sky and Sky standard deviation images. The options described in this section allow you to identify them. If you use the default output of NoiseChisel (see @ref{NoiseChisel output}) you don't have to worry about any of these options and just give NoiseChisel's output file to MakeCatalog as described in @ref{Invoking astmkcatalog}. @table @option @item -O STR @itemx --objectsfile=STR The file name of the object labels image, if the image is in another extension of the input file, calling this option is not mandatory, just specify the extension/HDU with the @option{--objectshdu} option. @item --objectshdu=STR The HDU/extension of the object labels image. Only pixels with values above zero will be considered. The objects label image has to be an integer data type (see @ref{Numeric data types}) and only pixels with a value larger than zero will be used. If this extension contains the @code{WCLUMPS} keyword with a value of @code{yes}, @code{1}, or @code{y} (not case sensitive), then MakeCatalog will also build a clumps catalog, see @ref{Invoking astmkcatalog}. @item -C STR @itemx --clumpsfile=STR Similar to @option{--objlabs} but for the labels of the clumps. This is only necessary if the image containing clump labels is not in the input file and the objects image has a @code{WCLUMPS} keyword, see @option{--objectshdu}. @item --clumpshdu=STR The HDU/extension of the object labels image. Only pixels with values above zero will be considered. The objects label image has to be an integer data type (see @ref{Numeric data types}) and only pixels with a value larger than zero will be used. @item -s STR @itemx --skyfile=STR File name of an image keeping the Sky value for each pixel. @item --skyhdu=STR The HDU of the Sky value image. @item -t STR @itemx --stdfile=STR File name of image keeping the Sky value standard deviation for each pixel. @item --stdhdu=STR The HDU of the Sky value standard deviation image. @end table @node MakeCatalog general settings, Upper-limit magnitude settings, MakeCatalog input files, Invoking astmkcatalog @subsubsection MakeCatalog general settings Some of the columns require particular settings (for example the zero point magnitude for measuring magnitudes), the options in this section can be used for such configurations. @table @option @item -z FLT @itemx --zeropoint=FLT The zero point magnitude for the input image, see @ref{Flux Brightness and magnitude}. @item -E @itemx --skysubtracted If the image has already been sky subtracted by another program, then you need to notify MakeCatalog through this option. Note that this is only relevant when the Signal to noise ratio is to be calculated. @item -T FLT @itemx --threshold=FLT For all the columns, only consider pixels that are above a given relative threshold. Symbolizing the value of this option as @mymath{T}, the Sky for a pixel at @mymath{(i,j)} with @mymath{\mu_{ij}} and its Standard deviation with @mymath{\sigma_{ij}}, that pixel will only be used if its value (@mymath{B_{ij}}) satisfies this condition: @mymath{B_{ij}>\mu_{ij}+{T}\sigma_{ij}}. The only calculations that will not be affected are is the average river values (@option{--riverave}), since they are used as a reference. A commented row will be added in the header of the output catalog that will print the given value, since this is a very important issue, it starts with @command{**IMPORTANT**}. NoiseChisel will detect very diffuse signal which is useful in most cases where the aggregate properties of the detections are desired, since there is signal there (with the desired certainty). However, in some cases, only the properties of the peaks of the objects/clumps are desired, for example in attempting to separate stars from galaxies, the peaks are the major target and the diffuse regions only act to complicate the separation. With this option, MakeCatalog will simply ignore any pixel below the relative threshold. @cindex NaN This option is not mandatory, so if it isn't given (after reading the command-line and all configuration files, see @ref{Configuration files}), MakeCatalog will still operate. However, if it has a value in any lower-level configuration file and you want to ignore that value for this particular run or in a higher-level configuration file, then set it to NaN, for example @option{--threshold=nan}. Gnuastro uses the C library's @code{strtod} function to read floats, which is not case-sensitive in reading NaN values. But to be consistent, it is good practice to only use @option{nan}. @item --nsigmag=FLT The median standard deviation (from the standard deviation image) will be multiplied by the value to this option and its magnitude will be reported in the comments of the output catalog. This value is a per-pixel value, not per object/clump and is not found over an area or aperture, like the common @mymath{5\sigma} values that are commonly reported as a measure of depth or the upper-limit measurements (see @ref{Quantifying measurement limits}). @end table @node Upper-limit magnitude settings, MakeCatalog output columns, MakeCatalog general settings, Invoking astmkcatalog @subsubsection Upper-limit magnitude settings The upper limit magnitude was discussed in @ref{Quantifying measurement limits}. Unlike other measured values/columns in MakeCatalog, the upper limit magnitude needs several defined parameters which are discussed here. All the upper limit magnitude specific options start with @option{up} for upper-limit, except for @option{--envseed} that is also present in other programs and is general for any job requiring random number generation (see @ref{Generating random numbers}). @cindex Reproducibility One very important consideration in Gnuastro is reproducibility. Therefore, the values to all of these parameters along with others (like the random number generator type and seed) are also reported in the comments of the final catalog when the upper limit magnitude column is desired. The random seed that is used to define the random positionings for each object or clump is unique and set based on the given seed, the total number of objects and clumps and also the labels of the clumps and objects. So with identical inputs, an identical upper-limit magnitude will be found. But even if the ordering of the object/clump labels differs (and the seed is the same) the result will not be the same. MakeCatalog will randomly place the object/clump footprint over the image and when the footprint doesn't fall on any object or masked region (see @option{--upmaskfile}) it will be used until the desired number (@option{--upnum}) of samples are found to estimate the distribution's standard deviation (see @ref{Quantifying measurement limits}). Otherwise it will be ignored and another random position will be generated. But when the profile is very large or the image is significantly covered by detections, it might not be possible to find the desired number of samplings. MakeProfiles will continue searching until 50 times the value given to @option{--upnum}. If @option{--upnum} good samples cannot be found until this limit, it will set the upper-limit magnitude for that object to NaN (blank). MakeCatalog will also print a warning if the range of positions available for the labeled region is smaller than double the size of the region. In such cases, the limited range of random positions can artificially decrease the standard deviation of the final distribution. @table @option @item --upmaskfile=STR File name of mask image to use for upper-limit calculation. In some cases (especially when doing matched photometry), the object labels specified in the main input and mask image might not be adequate. In other words they do not necessarily have to cover @emph{all} detected objects: the user might have selected only a few of the objects in their labeled image. This option can be used to ignore regions in the image in these situations when estimating the upper-limit magnitude. All the non-zero pixels of the image specified by this option (in the @option{--upmaskhdu} extension) will be ignored in the upper-limit magnitude measurements. For example, when you are using labels from another image, you can give NoiseChisel's objects image output for this image as the value to this option. In this way, you can be sure that regions with data do not harm your distribution. See @ref{Quantifying measurement limits} for more on the upper limit magnitude. @item --upmaskhdu=STR The extension in the file specified by @option{--upmask}. @item --upnum=INT The number of random samples to take for all the objects. A larger value to this option will give a more accurate result (asymptotically), but it will also slow down the process. When a randomly positioned sample overlaps with a detected/masked pixel it is not counted and another random position is found until the object completely lies over an undetected region. So you can be sure that for each object, this many samples over undetected objects are made. See the upper limit magnitude discussion in @ref{Quantifying measurement limits} for more. @item --uprange=INT,INT The range/width of the region (in pixels) to do random sampling along each dimension of the input image around each object's position. This is not a mandatory option and if not given (or given a value of zero in a dimension), the full possible range of the dataset along that dimension will be used. This is useful when the noise properties of the dataset vary gradually. In such cases, using the full range of the input dataset is going to bias the result. However, note that decreasing the the range of available positions too much will also artificially decrease the standard deviation of the final distribution (and thus bias the upper-limit measurement). @item --envseed Read the random number generator type and seed value from the environment (see @ref{Generating random numbers}). Random numbers are used in calculating the random positions of different samples of each object. @item --upsigmaclip=FLT,FLT The raw distribution of random values will not be used to find the upper-limit magnitude, it will first be @mymath{\sigma}-clipped (see @ref{Sigma clipping}) to avoid outliers in the distribution (mainly the faint undetected wings of bright/large objects in the image). This option takes two values: the first is the multiple of @mymath{\sigma}, and the second is the termination criteria. If the latter is larger than 1, it is read as an integer number and will be the number of times to clip. If it is smaller than 1, it is interpretted as the tolerance level to stop clipping. See @ref{Sigma clipping} for a complete explanation. @item --upnsigma=FLT The multiple of the final (@mymath{\sigma}-clipped) standard deviation (or @mymath{\sigma}) used to measure the upper-limit brightness or magnitude. @end table @node MakeCatalog output columns, , Upper-limit magnitude settings, Invoking astmkcatalog @subsubsection MakeCatalog output columns The final group of options particular to MakeCatalog are those that specify which columns should be written into the final output table. For each column there is an option, if it has been called on the command line or in any of the configuration files, it will included as a column in the output catalog in the same order (see @ref{Configuration file precedence}). Some of the columns apply to both objects and clumps and some are particular to only one of them. The latter cases are explicitly marked with [Objects] or [Clumps] to specify the catalog they will be placed in. @table @option @item --i @itemx --ids This is a unique option which can add multiple columns to the final catalog(s). Calling this option will put the object IDs (@option{--objid}) in the objects catalog and host-object-ID (@option{--hostobjid}) and ID-in-host-object (@option{--idinhostobj}) into the clumps catalog. Hence if only object catalogs are required, it has the same effect as @option{--objid}. @item --objid [Objects] ID of this object. @item -j @itemx --hostobjid [Clumps] The ID of the object which hosts this clump. @item --idinhostobj [Clumps] The ID of this clump in its host object. @item -C @itemx --numclumps [Objects] The number of clumps in this object. @item -a @itemx --area The raw area (number of pixels) in any clump or object independent of what pixel it lies over (if it is NaN/blank or unused for example). @item --clumpsarea [Objects] The total area of all the clumps in this object. @item --weightarea The area (number of pixels) used in the flux weighted position calculations. @item -x @itemx --x The flux weighted center of all objects and clumps along the first FITS axis (horizontal when viewed in SAO ds9), see @mymath{\overline{x}} in @ref{Measuring elliptical parameters}. The weight has to have a positive value (pixel value larger than the Sky value) to be meaningful! Specially when doing matched photometry, this might not happen: no pixel value might be above the Sky value. For such detections, the geometric center will be reported in this column (see @option{--geox}). You can use @option{--weightarea} to see which was used. @item -y @itemx --y The flux weighted center of all objects and clumps along the second FITS axis (vertical when viewed in SAO ds9). See @option{--x}. @item --geox The geometric center of all objects and clumps along the first FITS axis axis. The geometric center is the average pixel positions irrespective of their pixel values. @item --geoy The geometric center of all objects and clumps along the second FITS axis axis, see @option{--geox}. @item --clumpsx [Objects] The flux weighted center of all the clumps in this object along the first FITS axis. See @option{--x}. @item --clumpsy [Objects] The flux weighted center of all the clumps in this object along the second FITS axis. See @option{--x}. @item --clumpsgeox [Objects] The geometric center of all the clumps in this object along the first FITS axis. See @option{--geox}. @item --clumpsgeoy [Objects] The geometric center of all the clumps in this object along the second FITS axis. See @option{--geox}. @item -r @itemx --ra Flux weighted right ascension of all objects or clumps, see @option{--x}. This is just an alias for one of the lower-level @option{--w1} or @option{--w2} options. Using the FITS WCS keywords (@code{CTYPE}), MakeCatalog will determine which axis corresponds to the right ascension. If no @code{CTYPE} keywords start with @code{RA}, an error will be printed when requesting this column and MakeCatalog will abort. @item -d @itemx --dec Flux weighted declination of all objects or clumps, see @option{--x}. This is just an alias for one of the lower-level @option{--w1} or @option{--w2} options. Using the FITS WCS keywords (@code{CTYPE}), MakeCatalog will determine which axis corresponds to the declination. If no @code{CTYPE} keywords start with @code{DEC}, an error will be printed when requesting this column and MakeCatalog will abort. @item --w1 Flux weighted first WCS axis of all objects or clumps, see @option{--x}. The first WCS axis is commonly used as right ascension in images. @item --w2 Flux weighted second WCS axis of all objects or clumps, see @option{--x}. The second WCS axis is commonly used as declination in images. @item --geow1 Geometric center in first WCS axis of all objects or clumps, see @option{--geox}. The first WCS axis is commonly used as right ascension in images. @item --geow2 Geometric center in second WCS axis of all objects or clumps, see @option{--geox}. The second WCS axis is commonly used as declination in images. @item --clumpsw1 [Objects] Flux weighted center in first WCS axis of all clumps in this object, see @option{--x}. The first WCS axis is commonly used as right ascension in images. @item --clumpsw2 [Objects] Flux weighted declination of all clumps in this object, see @option{--x}. The second WCS axis is commonly used as declination in images. @item --clumpsgeow1 [Objects] Geometric center right ascension of all clumps in this object, see @option{--geox}. The first WCS axis is commonly used as right ascension in images. @item --clumpsgeow2 [Objects] Geometric center declination of all clumps in this object, see @option{--geox}. The second WCS axis is commonly used as declination in images. @item -b @itemx --brightness The brightness (sum of all pixel values), see @ref{Flux Brightness and magnitude}. For clumps, the ambient brightness (flux of river pixels around the clump multiplied by the area of the clump) is removed, see @option{--riverflux}. So the sum of clump brightnesses in the clump catalog will be smaller than the total clump brightness in the @option{--clumpbrightness} column of the objects catalog. If no usable pixels (blank or below the threshold) are present over the clump or object, the stored value will be NaN (note that zero is meaningful). @item --clumpbrightness [Objects] The total brightness of the clumps within an object. This is simply the sum of the pixels associated with clumps in the object. If no usable pixels (blank or below the threshold) are present over the clump or object, the stored value will be NaN, because zero (note that zero is meaningful). @item --noriverbrightness [Clumps] The Sky (not river) subtracted clump brightness. By definition, for the clumps, the average brightness of the rivers surrounding it are subtracted from it for a first order accounting for contamination by neighbors. In cases where you will be calculating the flux brightness difference later (one example below) the contamination will be (mostly) removed at that stage, which is why this column was added. One example might be this: you want to know the change in the clump flux as a function of threshold (see @option{--threshold}). So you will make two catalogs (each having this column but with different thresholds) and then subtract the lower threshold catalog (higher brightness) from the higher threshold catalog (lower brightness). The effect is most visible when the rivers have a high average signal-to-noise ratio. The removed contribution from the pixels below the threshold will be less than the river pixels. Therefore the river-subtracted brightness (@option{--brightness}) for the thresholded catalog for such clumps will be larger than the brightness with no threshold! If no usable pixels (blank or below the possibly given threshold) are present over the clump or object, the stored value will be NaN (note that zero is meaningful). @item -m @itemx --magnitude The magnitude of clumps or objects, see @option{--brightness}. @item -e @itemx --magnitudeerr The magnitude error of clumps or objects. The magnitude error is calculated from the signal-to-noise ratio (see @option{--sn} and @ref{Quantifying measurement limits}). Note that until now this error assumes un-correlated pixel values and also does not include the error in estimating the aperture (or error in generating the labeled image). For now these factors have to be found by other means. @url{https://savannah.gnu.org/task/index.php?14124, Task 14124} has been defined for work on adding these sources of error too. @item --clumpsmagnitude [Objects] The magnitude of all clumps in this object, see @option{--clumpbrightness}. @item --upperlimit The upper limit value (in units of the input image) for this object or clump. See @ref{Quantifying measurement limits} and @ref{Upper-limit magnitude settings} for a complete explanation. This is very important for the fainter and smaller objects in the image where the measured magnitudes are not reliable. @item --upperlimitmag The upper limit magnitude for this object or clump. See @ref{Quantifying measurement limits} and @ref{Upper-limit magnitude settings} for a complete explanation. This is very important for the fainter and smaller objects in the image where the measured magnitudes are not reliable. @item --riverave [Clumps] The average brightness of the river pixels around this clump. River pixels were defined in Akhlaghi and Ichikawa 2015. In short they are the pixels immediately outside of the clumps. This value is used internally to find the brightness (or magnitude) and signal to noise ratio of the clumps. It can generally also be used as a scale to gauge the base (ambient) flux surrounding the clump. In case there was no river pixels, then this column will have the value of the Sky under the clump. So note that this value is @emph{not} sky subtracted. @item --rivernum [Clumps] The number of river pixels around this clump, see @option{--riverflux}. @item -n @itemx --sn The Signal to noise ratio (S/N) of all clumps or objects. See Akhlaghi and Ichikawa (2015) for the exact equations used. @item --sky The sky flux (per pixel) value under this object or clump. This is actually the mean value of all the pixels in the sky image that lie on the same position as the object or clump. @item --std The sky value standard deviation (per pixel) for this clump or object. Like @option{--sky}, this is the average of the values in the input sky standard deviation image pixels that lie over this object. @item -A @itemx --semimajor The pixel-value weighted semi-major axis of the profile (assuming it is an ellipse) in units of pixels. See @ref{Measuring elliptical parameters}. @item -B @itemx --semiminor The pixel-value weighted semi-minor axis of the profile (assuming it is an ellipse) in units of pixels. See @ref{Measuring elliptical parameters}. @item -p @itemx --positionangle The pixel-value weighted angle of the semi-major axis with the first FITS axis in degrees. See @ref{Measuring elliptical parameters}. @item --geosemimajor The geometric (ignoring pixel values) semi-major axis of the profile, assuming it is an ellipse. @item --geosemiminor The geometric (ignoring pixel values) semi-minor axis of the profile, assuming it is an ellipse. @item --geopositionangle The geometric (ignoring pixel values) angle of the semi-major axis with the first FITS axis in degrees. @end table @node Match, , MakeCatalog, Data analysis @section Match Data can come come from different telescopes, filters, software and even different configurations for a single software. As a result, one of the primary things to do after generating catalogs from each of these sources (for example with @ref{MakeCatalog}), is to find which sources in one catalog correspond to which in the other(s). In other words, to `match' the two catalogs with each other. Gnuastro's Match program is in charge of such operations. The nearest objects in the two catalogs, within the given aperture, will be found and given as output. The aperture can be a circle or an ellipse with any orientation. @menu * Invoking astmatch:: Inputs, outputs and options of Match @end menu @node Invoking astmatch, , Match, Match @subsection Invoking Match When given two catalogs, Match finds the rows that are nearest to each other within an input aperture. The executable name is @file{astmatch} with the following general template @example $ astmatch [OPTION ...] input-1 input-2 @end example @noindent One line examples: @example ## 1D wavelength match (within 5 angstroms) of the two inputs. ## The wavelengths are in the 5th and 10th columns respectively. $ astmatch --aperture=5e-10 --ccol1=5 --ccol2=10 in1.fits in2.txt ## Match the two catalogs with a circular aperture of width 2. ## (Units same as given positional columns). ## (By default two columns are given for `--ccol1' and `--ccol2', ## The number of values to these determines the dimensions). $ astmatch --aperture=2 input1.txt input2.fits ## Similar to before, but the output is created by merging various ## columns from the two inputs: columns 1, RA, DEC from the first ## input, followed by all columns starting with MAG and the 8th ## column from second input and finally the 10th from first input. $ astmatch --aperture=2 input1.txt input2.fits \ --outcols=a1,aRA,aDEC,b/^MAG/,bBRG,a10 ## Match the two catalogs within an elliptical aperture of 1 and 2 ## arcseconds along RA and Dec respectively. $ astmatch --aperture=1/3600,2/3600 in1.fits in2.txt ## Match the RA and DEC columns of the first input with the RA_D ## and DEC_D columns of the second within a 0.5 arcseconds aperture. $ astmatch --ccol1=RA,DEC --ccol2=RA_D,DEC_D --aperture0.5/3600 \ in1.fits in2.fits @end example Two inputs are necessary for Match to start processing. The inputs can be plain text tables or FITS tables, see @ref{Tables}. Match follows the same basic behavior of all Gnuastro programs as fully described in @ref{Common program behavior}. If the first input is a FITS file, the common @option{--hdu} option (see @ref{Input output options}) should be used to identify the extension. When the second input is FITS, the extension must be specified with @option{--hdu2}. When @option{--quiet} is not called, Match will print the number of matches found in standard output (on the command-line). If no match was found, no output file will be created (table or log file). When matches are found, by default, the output file(s) will be the re-arranged input tables such that the rows match each other: both output tables will have the same number of rows which are matched with each other. If @option{--outcols} is called, the output is a single table with rows chosen from either of the two inputs in any order, see the description of @option{--outcols}. If the @option{--logasoutput} option is called, the output will be a single table with the contents of the log file, see below. If no output file name is given with the @option{--output} option, then automatic output @ref{Automatic output} will be used to determine the output name(s). Depending on @option{--tableformat} (see @ref{Input output options}), the output will then be a (possibly multi-extension) FITS file or (possibly two) plain text file(s). When the output is a FITS file, the default re-arranged inputs will be two extensions of the output FITS file. With @option{--outcols} and @option{--logasoutput}, the FITS output will be a single table (in one extension). When the @option{--log} option is called (see @ref{Operating mode options}), Match will also create a file named @file{astmatch.fits} (or @file{astmatch.txt}, depending on @option{--tableformat}, see @ref{Input output options}) in the directory it is run in. This log table will have three columns. The first and second columns show the matching row/record number (counting from 1) of the first and second input catalogs respectively. The third column is the distance between the two matched positions. The units of the distance are the same as the given coordinates (given the possible ellipticity, see description of @option{--aperture} below). When @option{--logasoutput} is called, no log file (with a fixed name) will be created. In this case, the output file (possibly given by the @option{--output} option) will have the contents of this log file. @table @option @item -H STR @itemx --hdu2=STR The extension/HDU of the second input if it is a FITS file. When it isn't a FITS file, this option's value is ignored. For the first input, the common option @option{--hdu} must be used. @item --outcols=STR Columns from both inputs to write into a single matched table output. The value to @code{--outcols} must be a comma-separated list of strings, for example @option{--outcols=a1,bRA,bDEC}. The first character of each string specifies the input catalog: @option{a} for the first and @option{b} for the second. The rest of the characters of the string will be directly used to identify the proper column(s) in the respective table. See @ref{Selecting table columns} for how columns can be specified in Gnuastro. In this example, the output will have three columns: the first column of the first input and the @option{RA} and @option{DEC} columns of the second input. Another example is given in the one-line examples above. Compared to the default case (where two tables with all their columns) are printed, using this option is much faster: it will only read and re-arrange the necessary columns and it will write a single output table. Combined with regular expressions in large tables, this can be a very powerful and convenient way to retrieve your desired information and do the match at the same time. @item -l @itemx --logasoutput The output file will have the contents of the log file: indexs in the two catalogs that match with each other along with their distance. See description above. When this option is called, a log file called @file{astmatch.txt} will not be created. With this option, the default output behavior (two tables containing the re-arranged inputs) will be @item --notmatched Write the non-matching rows into the outputs, not the matched ones. Note that with this option, the two output tables will not necessarily have the same number of rows. Therefore, this option cannot be called with @option{--outcols}. @option{--outcols} prints mixed columns from both inputs, so they must all have the same number of elements and must correspond to each other. @item -c INT/STR[,INT/STR] @itemx --ccol1=INT/STR[,INT/STR] The coordinate columns of the first input. The number of dimensions for the match is determined by the number of comma-separated values given to this option. The values can be the column number (counting from 1), exact column name or a regular expression. For more, see @ref{Selecting table columns}. See the one-line examples above for some usages of this option. @item -C INT/STR[,INT/STR] @itemx --ccol2=INT/STR[,INT/STR] The coordinate columns of the second input. See the example in @option{--ccol1} for more. @item -a FLT[,FLT[,FLT]] @itemx --aperture=FLT[,FLT[,FLT]] Parameters of the aperture for matching. The values given to this option can be fractions, for example when the position columns are in units of degrees, @option{1/3600} can be used to ask for one arcsecond. The interpretation of the values depends on the requested dimensions (determined from @option{--ccol1} and @code{--ccol2}) and how many values are given to this option. @table @asis @item 1D match The aperture/interval can only take one value: half of the interval around each point (maximum distance from each point). @item 2D match In a 2D match, the aperture can be a circle, an ellipse aligned in the axes or an ellipse with a rotated major axis. To simply the usage, you can determine the shape based on the number of free parameters for each. @table @asis @item 1 number For example @option{--aperture=2}. The aperture will be a circle of the given radius. The value will be in the same units as the columns in @option{--ccol1} and @option{--ccol2}). @item 2 numbers For example @option{--aperture=3,4e-10}. The aperture will be an ellipse (if the two numbers are different) with the respective value along each dimension. The numbers are in units of the first and second axis. In the example above, the semi-axis value along the first axis will be 3 (in units of the first coordinate) and along the second axis will be @mymath{4\times10^{-10}} (in units of the second coordinate). Such values can happen if you are comparing catalogs of a spectra for example. If more than one object exists in the aperture, the nearest will be found along the major axis as described in @ref{Defining an ellipse}. @item 3 numbers For example @option{--aperture=2,0.6,30}. The aperture will be an ellipse (if the second value is not 1). The first number is the semi-major axis, the second is the axis ratio and the third is the position angle (in degrees). If multiple matches are found within the ellipse, the distance (to find the nearest) is calculated along the major axis in the elliptical space, see @ref{Defining an ellipse}. @end table @end table @end table @node Modeling and fittings, High-level calculations, Data analysis, Top @chapter Modeling and fitting @cindex Fitting @cindex Modeling In order to fully understand observations after initial analysis on the image, it is very important to compare them with the existing models to be able to further understand both the models and the data. The tools in this chapter create model galaxies and will provide 2D fittings to be able to understand the detections. @menu * MakeProfiles:: Making mock galaxies and stars. * MakeNoise:: Make (add) noise to an image. @end menu @node MakeProfiles, MakeNoise, Modeling and fittings, Modeling and fittings @section MakeProfiles @cindex Checking detection algorithms @pindex @r{MakeProfiles (}astmkprof@r{)} MakeProfiles will create mock astronomical profiles from a catalog, either individually or together in one output image. In data analysis, making a mock image can act like a calibration tool, through which you can test how successfully your detection technique is able to detect a known set of objects. There are commonly two aspects to detecting: the detection of the fainter parts of bright objects (which in the case of galaxies fade into the noise very slowly) or the complete detection of an over-all faint object. Making mock galaxies is the most accurate (and idealistic) way these two aspects of a detection algorithm can be tested. You also need mock profiles in fitting known functional profiles with observations. MakeProfiles was initially built for extra galactic studies, so currently the only astronomical objects it can produce are stars and galaxies. We welcome the simulation of any other astronomical object. The general outline of the steps that MakeProfiles takes are the following: @enumerate @item Build the full profile out to its truncation radius in a possibly over-sampled array. @item Multiply all the elements by a fixed constant so its total magnitude equals the desired total magnitude. @item If @option{--individual} is called, save the array for each profile to a FITS file. @item If @option{--nomerged} is not called, add the overlapping pixels of all the created profiles to the output image and abort. @end enumerate Using input values, MakeProfiles adds the World Coordinate System (WCS) headers of the FITS standard to all its outputs (except PSF images!). For a simple test on a set of mock galaxies in one image, there is no need for the third step or the WCS information. @cindex Transform image @cindex Lensing simulations @cindex Image transformations However in complicated simulations like weak lensing simulations, where each galaxy undergoes various types of individual transformations based on their position, those transformations can be applied to the different individual images with other programs. After all the transformations are applied, using the WCS information in each individual profile image, they can be merged into one output image for convolution and adding noise. @menu * Modeling basics:: Astronomical modeling basics. * If convolving afterwards:: Considerations for convolving later. * Flux Brightness and magnitude:: About these measures of energy. * Profile magnitude:: Definition of total profile magnitude. * Invoking astmkprof:: Inputs and Options for MakeProfiles. @end menu @node Modeling basics, If convolving afterwards, MakeProfiles, MakeProfiles @subsection Modeling basics In the subsections below, first a review of some very basic information and concepts behind modeling a real astronomical image is given. You can skip this subsection if you are already sufficiently familiar with these concepts. @menu * Defining an ellipse:: An ellipse on a pixelated grid. * PSF:: Radial profiles for the PSF. * Stars:: Making mock star profiles. * Galaxies:: Radial profiles for galaxies. * Sampling from a function:: Sample a function on a pixelated canvas. * Oversampling:: Oversampling the model. @end menu @node Defining an ellipse, PSF, Modeling basics, Modeling basics @subsubsection Defining an ellipse @cindex Ellipse @cindex Axis ratio @cindex Position angle The PSF, see @ref{PSF}, and galaxy radial profiles are generally defined on an ellipse. Therefore, in this section we'll start defining an ellipse on a pixelated 2D surface. Labeling the major axis of an ellipse @mymath{a}, and its minor axis with @mymath{b}, the @emph{axis ratio} is defined as: @mymath{q\equiv b/a}. The major axis of an ellipse can be aligned in any direction, therefore the angle of the major axis with respect to the horizontal axis of the image is defined to be the @emph{position angle} of the ellipse and in this book, we show it with @mymath{\theta}. @cindex Radial profile on ellipse Our aim is to put a radial profile of any functional form @mymath{f(r)} over an ellipse. Hence we need to associate a radius/distance to every point in space. Let's define the radial distance @mymath{r_{el}} as the distance on the major axis to the center of an ellipse which is located at @mymath{i_c} and @mymath{j_c} (in other words @mymath{r_{el}\equiv{a}}). We want to find @mymath{r_{el}} of a point located at @mymath{(i,j)} (in the image coordinate system) from the center of the ellipse with axis ratio @mymath{q} and position angle @mymath{\theta}. First the coordinate system is rotated@footnote{Do not confuse the signs of @mymath{sin} with the rotation matrix defined in @ref{Warping basics}. In that equation, the point is rotated, here the coordinates are rotated and the point is fixed.} by @mymath{\theta} to get the new rotated coordinates of that point @mymath{(i_r,j_r)}: @dispmath{i_r(i,j)=+(i_c-i)\cos\theta+(j_c-j)\sin\theta} @dispmath{j_r(i,j)=-(i_c-i)\sin\theta+(j_c-j)\cos\theta} @cindex Elliptical distance @noindent Recall that an ellipse is defined by @mymath{(i_r/a)^2+(j_r/b)^2=1} and that we defined @mymath{r_{el}\equiv{a}}. Hence, multiplying all elements of the the ellipse definition with @mymath{r_{el}^2} we get the elliptical distance at this point point located: @mymath{r_{el}=\sqrt{i_r^2+(j_r/q)^2}}. To place the radial profiles explained below over an ellipse, @mymath{f(r_{el})} is calculated based on the functional radial profile desired. @cindex Breadth first search @cindex Inside-out construction @cindex Making profiles pixel by pixel @cindex Pixel by pixel making of profiles MakeProfiles builds the profile starting from the nearest element (pixel in an image) in the dataset to the profile center. The profile value is calculated for that central pixel using monte carlo integration, see @ref{Sampling from a function}. The next pixel is the next nearest neighbor to the central pixel as defined by @mymath{r_{el}}. This process goes on until the profile is fully built upto the trunctation radius. This is done fairly efficiently using a breadth first parsing strategy@footnote{@url{http://en.wikipedia.org/wiki/Breadth-first_search}} which is implemented through an ordered linked list. Using this approach, we build the profile by expanding the circumference. Not one more extra pixel has to be checked (the calculation of @mymath{r_{el}} from above is not cheap in CPU terms). Another consequence of this strategy is that extending MakeProfiles to three dimensions becomes very simple: only the neighbors of each pixel have to be changed. Everything else after that (when the pixel index and its radial profile have entered the linked list) is the same, no matter the number of dimensions we are dealing with. @node PSF, Stars, Defining an ellipse, Modeling basics @subsubsection Point Spread Function @cindex PSF @cindex Point source @cindex Diffraction limited @cindex Point Spread Function @cindex Spread of a point source Assume we have a `point' source, or a source that is far smaller than the maximum resolution (a pixel). When we take an image of it, it will `spread' over an area. To quantify that spread, we can define a `function'. This is how the point spread function or the PSF of an image is defined. This `spread' can have various causes, for example in ground based astronomy, due to the atmosphere. In practice we can never surpass the `spread' due to the diffraction of the lens aperture. Various other effects can also be quantified through a PSF. For example, the simple fact that we are sampling in a discrete space, namely the pixels, also produces a very small `spread' in the image. @cindex Blur image @cindex Convolution @cindex Image blurring @cindex PSF image size Convolution is the mathematical process by which we can apply a `spread' to an image, or in other words blur the image, see @ref{Convolution process}. The Brightness of an object should remain unchanged after convolution, see @ref{Flux Brightness and magnitude}. Therefore, it is important that the sum of all the pixels of the PSF be unity. The PSF image also has to have an odd number of pixels on its sides so one pixel can be defined as the center. In MakeProfiles, the PSF can be set by the two methods explained below. @table @asis @item Parametric functions @cindex FWHM @cindex PSF width @cindex Parametric PSFs @cindex Full Width at Half Maximum A known mathematical function is used to make the PSF. In this case, only the parameters to define the functions are necessary and MakeProfiles will make a PSF based on the given parameters for each function. In both cases, the center of the profile has to be exactly in the middle of the central pixel of the PSF (which is automatically done by MakeProfiles). When talking about the PSF, usually, the full width at half maximum or FWHM is used as a scale of the width of the PSF. @table @cite @item Gaussian @cindex Gaussian distribution In the older papers, and to a lesser extent even today, some researchers use the 2D Gaussian function to approximate the PSF of ground based images. In its most general form, a Gaussian function can be written as: @dispmath{f(r)=a \exp \left( -(x-\mu)^2 \over 2\sigma^2 \right)+d} Since the center of the profile is pre-defined, @mymath{\mu} and @mymath{d} are constrained. @mymath{a} can also be found because the function has to be normalized. So the only important parameter for MakeProfiles is the @mymath{\sigma}. In the Gaussian function we have this relation between the FWHM and @mymath{\sigma}: @cindex Gaussian FWHM @dispmath{\rm{FWHM}_g=2\sqrt{2\ln{2}}\sigma \approx 2.35482\sigma} @item Moffat @cindex Moffat function The Gaussian profile is much sharper than the images taken from stars on photographic plates or CCDs. Therefore in 1969, Moffat proposed this functional form for the image of stars: @dispmath{f(r)=a \left[ 1+\left( r\over \alpha \right)^2 \right]^{-\beta}} @cindex Moffat beta Again, @mymath{a} is constrained by the normalization, therefore two parameters define the shape of the Moffat function: @mymath{\alpha} and @mymath{\beta}. The radial parameter is @mymath{\alpha} which is related to the FWHM by @cindex Moffat FWHM @dispmath{\rm{FWHM}_m=2\alpha\sqrt{2^{1/\beta}-1}} @cindex Compare Moffat and Gaussian @cindex PSF, Moffat compared Gaussian @noindent Comparing with the PSF predicted from atmospheric turbulence theory with a Moffat function, Trujillo et al.@footnote{Trujillo, I., J. A. L. Aguerri, J. Cepa, and C. M. Gutierrez (2001). ``The effects of seeing on S@'ersic profiles - II. The Moffat PSF''. In: MNRAS 328, pp. 977---985.} claim that @mymath{\beta} should be 4.765. They also show how the Moffat PSF contains the Gaussian PSF as a limiting case when @mymath{\beta\to\infty}. @end table @item An input FITS image An input image file can also be specified to be used as a PSF. If the sum of its pixels are not equal to 1, the pixels will be multiplied by a fraction so the sum does become 1. @end table While the Gaussian is only dependent on the FWHM, the Moffat function is also dependent on @mymath{\beta}. Comparing these two functions with a fixed FWHM gives the following results: @itemize @item Within the FWHM, the functions don't have significant differences. @item For a fixed FWHM, as @mymath{\beta} increases, the Moffat function becomes sharper. @item The Gaussian function is much sharper than the Moffat functions, even when @mymath{\beta} is large. @end itemize @node Stars, Galaxies, PSF, Modeling basics @subsubsection Stars @cindex Modeling stars @cindex Stars, modeling In MakeProfiles, stars are generally considered to be a point source. This is usually the case for extra galactic studies, were nearby stars are also in the field. Since a star is only a point source, we assume that it only fills one pixel prior to convolution. In fact, exactly for this reason, in astronomical images the light profiles of stars are one of the best methods to understand the shape of the PSF and a very large fraction of scientific research is preformed by assuming the shapes of stars to be the PSF of the image. @node Galaxies, Sampling from a function, Stars, Modeling basics @subsubsection Galaxies @cindex Galaxy profiles @cindex S@'ersic profile @cindex Profiles, galaxies @cindex Generalized de Vaucouleur profile Today, most practitioners agree that the flux of galaxies can be modeled with one or a few generalized de Vaucouleur's (or S@'ersic) profiles. @dispmath{I(r) = I_e \exp \left ( -b_n \left[ \left( r \over r_e \right)^{1/n} -1 \right] \right )} @cindex Brightness @cindex S@'ersic, J. L. @cindex S@'ersic index @cindex Effective radius @cindex Radius, effective @cindex de Vaucouleur profile @cindex G@'erard de Vaucouleurs G@'erard de Vaucouleurs (1918-1995) was first to show in 1948 that this function best fits the galaxy light profiles, with the only difference that he held @mymath{n} fixed to a value of 4. 20 years later in 1968, J. L. S@'ersic showed that @mymath{n} can have a variety of values and does not necessarily need to be 4. This profile depends on the effective radius (@mymath{r_e}) which is defined as the radius which contains half of the profile brightness (see @ref{Profile magnitude}). @mymath{I_e} is the flux at the effective radius. The S@'ersic index @mymath{n} is used to define the concentration of the profile within @mymath{r_e} and @mymath{b_n} is a constant dependent on @mymath{n}. MacArthur et al.@footnote{MacArthur, L. A., S. Courteau, and J. A. Holtzman (2003). ``Structure of Disk-dominated Galaxies. I. Bulge/Disk Parameters, Simulations, and Secular Evolution''. In: ApJ 582, pp. 689---722.} show that for @mymath{n>0.35}, @mymath{b_n} can be accurately approximated using this equation: @dispmath{b_n=2n - {1\over 3} + {4\over 405n} + {46\over 25515n^2} + {131\over 1148175n^3}-{2194697\over 30690717750n^4}} @node Sampling from a function, Oversampling, Galaxies, Modeling basics @subsubsection Sampling from a function @cindex Sampling A pixel is the ultimate level of accuracy to gather data, we can't get any more accurate in one image, this is known as sampling in signal processing. However, the mathematical profiles which describe our models have infinite accuracy. Over a large fraction of the area of astrophysically interesting profiles (for example galaxies or PSFs), the variation of the profile over the area of one pixel is not too significant. In such cases, the elliptical radius (@mymath{r_{el}} of the center of the pixel can be assigned as the final value of the pixel, see @ref{Defining an ellipse}). @cindex Integration over pixel @cindex Gradient over pixel area @cindex Function gradient over pixel area As you approach their center, some galaxies become very sharp (their value significantly changes over one pixel's area). This sharpness increases with smaller effective radius and larger S@'ersic values. Thus rendering the central value extremely inaccurate. The first method that comes to mind for solving this problem is integration. The functional form of the profile can be integrated over the pixel area in a 2D integration process. However, unfortunately numerical integration techniques also have their limitations and when such sharp profiles are needed they can become extremely inaccurate. @cindex Monte carlo integration The most accurate method of sampling a continuous profile on a discrete space is by choosing a large number of random points within the boundaries of the pixel and taking their average value (or Monte Carlo integration). This is also, generally speaking, what happens in practice with the photons on the pixel. The number of random points can be set with @option{--numrandom}. Unfortunately, repeating this Monte Carlo process would be extremely time and CPU consuming if it is to be applied to every pixel. In order to not loose too much accuracy, in MakeProfiles, the profile is built using both methods explained below. The building of the profile begins from its central pixel and continues (radially) outwards. Monte Carlo integration is first applied (which yields @mymath{F_r}), then the central pixel value (@mymath{F_c}) is calculated on the same pixel. If the fractional difference (@mymath{|F_r-F_c|/F_r}) is lower than a given tolerance level (specified with @option{--tolerance}) MakeProfiles will stop using Monte Carlo integration and only use the central pixel value. @cindex Inside-out construction The ordering of the pixels in this inside-out construction is based on @mymath{r=\sqrt{(i_c-i)^2+(j_c-j)^2}}, not @mymath{r_{el}}, see @ref{Defining an ellipse}. When the axis ratios are large (near one) this is fine. But when they are small and the object is highly elliptical, it might seem more reasonable to follow @mymath{r_{el}} not @mymath{r}. The problem is that the gradient is stronger in pixels with smaller @mymath{r} (and larger @mymath{r_{el}}) than those with smaller @mymath{r_{el}}. In other words, the gradient is strongest along the minor axis. So if the next pixel is chosen based on @mymath{r_{el}}, the tolerance level will be reached sooner and lots of pixels with large fractional differences will be missed. Monte Carlo integration uses a random number of points. Thus, every time you run it, by default, you will get a different distribution of points to sample within the pixel. In the case of large profiles, this will result in a slight difference of the pixels which use Monte Carlo integration each time MakeProfiles is run. To have a deterministic result, you have to fix the random number generator properties which is used to build the random distribution. This can be done by setting the @code{GSL_RNG_TYPE} and @code{GSL_RNG_SEED} environment variables and calling MakeProfiles with the @option{--envseed} option. To learn more about the process of generating random numbers, see @ref{Generating random numbers}. The seed values are fixed for every profile: with @option{--envseed}, all the profiles have the same seed and without it, each will get a different seed using the system clock (which is accurate to within one microsecond). The same seed will be used to generate a random number for all the sub-pixel positions of all the profiles. So in the former, the sub-pixel points checked for all the pixels undergoing Monte carlo integration in all profiles will be identical. In other words, the sub-pixel points in the first (closest to the center) pixel of all the profiles will be identical with each other. All the second pixels studied for all the profiles will also receive an identical (different from the first pixel) set of sub-pixel points and so on. As long as the number of random points used is large enough or the profiles are not identical, this should not cause any systematic bias. @node Oversampling, , Sampling from a function, Modeling basics @subsubsection Oversampling @cindex Oversampling The steps explained in @ref{Sampling from a function} do give an accurate representation of a profile prior to convolution. However, in an actual observation, the image is first convolved with or blurred by the atmospheric and instrument PSF in a continuous space and then it is sampled on the discrete pixels of the camera. @cindex PSF over-sample In order to more accurately simulate this process, the un-convolved image and the PSF are created on a finer pixel grid. In other words, the output image is a certain odd-integer multiple of the desired size, we can call this `oversampling'. The user can specify this multiple as a command-line option. The reason this has to be an odd number is that the PSF has to be centered on the center of its image. An image with an even number of pixels on each side does not have a central pixel. The image can then be convolved with the PSF (which should also be oversampled on the same scale). Finally, image can be sub-sampled to get to the initial desired pixel size of the output image. After this, mock noise can be added as explained in the next section. This is because unlike the PSF, the noise occurs in each output pixel, not on a continuous space like all the prior steps. @node If convolving afterwards, Flux Brightness and magnitude, Modeling basics, MakeProfiles @subsection If convolving afterwards In case you want to convolve the image later with a given point spread function, make sure to use a larger image size. After convolution, the profiles become larger and a profile that is normally completely outside of the image might fall within it. On one axis, if you want your final (convolved) image to be @mymath{m} pixels and your PSF is @mymath{2n+1} pixels wide, then when calling MakeProfiles, set the axis size to @mymath{m+2n}, not @mymath{m}. You also have to shift all the pixel positions of the profile centers on the that axis by @mymath{n} pixels to the positive. After convolution, you can crop the outer @mymath{n} pixels with the section crop box specification of Crop: @option{--section=n:*-n,n:*-n} assuming your PSF is a square, see @ref{Crop section syntax}. This will also remove all discrete Fourier transform artifacts (blurred sides) from the final image. To facilitate this shift, MakeProfiles has the options @option{--xshift}, @option{--yshift} and @option{--prepforconv}, see @ref{Invoking astmkprof}. @node Flux Brightness and magnitude, Profile magnitude, If convolving afterwards, MakeProfiles @subsection Flux Brightness and magnitude @cindex ADU @cindex Gain @cindex Counts Astronomical data pixels are usually in units of counts@footnote{Counts are also known as analog to digital units (ADU).} or electrons or either one divided by seconds. To convert from the counts to electrons, you will need to know the instrument gain. In any case, they can be directly converted to energy or energy/time using the basic hardware (telescope, camera and filter) information. We will continue the discussion assuming the pixels are in units of energy/time. @cindex Flux @cindex Luminosity @cindex Brightness The @emph{brightness} of an object is defined as its total detected energy per time. This is simply the sum of the pixels that are associated with that detection by our detection tool for example @ref{NoiseChisel}@footnote{If further processing is done, for example the Kron or Petrosian radii are calculated, then the detected area is not sufficient and the total area that was within the respective radius must be used.}. The @emph{flux} of an object is in units of energy/time/area and for a detected object, it is defined as its brightness divided by the area used to collect the light from the source or the telescope aperture (for example in @mymath{cm^2})@footnote{For a full object that spans over several pixels, the telescope area should be used to find the flux. However, sometimes, only the brightness per pixel is desired. In such cases this book also @emph{loosely} uses the term flux. This is only approximately accurate however, since while all the pixels have a fixed area, the pixel size can vary with camera on the telescope.}. Knowing the flux (@mymath{f}) and distance to the object (@mymath{r}), we can calculate its @emph{luminosity}: @mymath{L=4{\pi}r^2f}. Therefore, flux and luminosity are intrinsic properties of the object, while brightness depends on our detecting tools (hardware and software). Here we will not be discussing luminosity, but brightness. However, since luminosity is the astrophysically interesting quantity, we also defined it here to avoid possible confusion between these two terms because they both have the same units. @cindex Magnitude zero-point @cindex Magnitudes from flux @cindex Flux to magnitude conversion @cindex Astronomical Magnitude system Images of astronomical objects span over a very large range of brightness. With the Sun (as the brightest object) being roughly @mymath{2.5^{60}=10^{24}} times brighter than the faintest galaxies we can currently detect. Therefore discussing brightness will be very hard, and astronomers have chosen to use a logarithmic scale to talk about the brightness of astronomical objects. But the logarithm can only be usable with a unit-less and always positive value. Fortunately brightness is always positive and to remove the units we divide the brightness of the object (@mymath{B}) by a reference brightness (@mymath{B_r}). We then define the resulting logarithmic scale as @mymath{magnitude} through the following relation@footnote{The @mymath{-2.5} factor in the definition of magnitudes is a legacy of the our ancient colleagues and in particular Hipparchus of Nicaea (190-120 BC).} @dispmath{m-m_r=-2.5\log_{10} \left( B \over B_r \right)} @cindex Zero-point magnitude @noindent @mymath{m} is defined as the magnitude of the object and @mymath{m_r} is the pre-defined magnitude of the reference brightness. One particularly easy condition is when @mymath{B_r=1}. This will allow us to summarize all the hardware specific parameters discussed above into one number as the reference magnitude which is commonly known as the Zero-point@footnote{When @mymath{B=Br=1}, the right side of the magnitude definition will be zero. Hence the name, ``zero-point''.} magnitude. @node Profile magnitude, Invoking astmkprof, Flux Brightness and magnitude, MakeProfiles @subsection Profile magnitude @cindex Brightness @cindex Truncation radius @cindex Sum for total flux To find the profile brightness or its magnitude, (see @ref{Flux Brightness and magnitude}), it is customary to use the 2D integration of the flux to infinity. However, in MakeProfiles we do not follow this idealistic approach and apply a more realistic method to find the total brightness or magnitude: the sum of all the pixels belonging to a profile within its predefined truncation radius. Note that if the truncation radius is not large enough, this can be significantly different from the total integrated light to infinity. @cindex Integration to infinity An integration to infinity is not a realistic condition because no galaxy extends indefinitely (important for high S@'ersic index profiles), pixelation can also cause a significant difference between the actual total pixel sum value of the profile and that of integration to infinity, especially in small and high S@'ersic index profiles. To be safe, you can specify a large enough truncation radius for such compact high S@'ersic index profiles. If oversampling is used then the brightness is calculated using the over-sampled image, see @ref{Oversampling} which is much more accurate. The profile is first built in an array completely bounding it with a normalization constant of unity (see @ref{Galaxies}). Taking @mymath{B} to be the desired brightness and @mymath{S} to be the sum of the pixels in the created profile, every pixel is then multiplied by @mymath{B/S} so the sum is exactly @mymath{B}. If the @option{--individual} option is called, this same array is written to a FITS file. If not, only the overlapping pixels of this array and the output image are kept and added to the output array. @node Invoking astmkprof, , Profile magnitude, MakeProfiles @subsection Invoking MakeProfiles MakeProfiles will make any number of profiles specified in a catalog either individually or in one image. The executable name is @file{astmkprof} with the following general template @example $ astmkprof [OPTION ...] [Catalog] @end example @noindent One line examples: @example ## Make an image with profiles in catalog.txt (with default size): $ astmkprof catalog.txt ## Make the profiles in catalog.txt over image.fits: $ astmkprof --background=image.fits catalog.txt ## Make a Moffat PSF with FWHM 3pix, beta=2.8, truncation=5 $ astmkprof --kernel=moffat,2.8,5 --oversample=1 ## Make profiles in catalog, using RA and Dec in the given column: $ astmkprof --ccol=RA_CENTER --ccol=DEC_CENTER --mode=wcs catalog.txt ## Make a 1500x1500 merged image (oversampled 500x500) image along ## with an individual image for all the profiles in catalog: $ astmkprof --individual --oversample 3 --naxis=500,500 catalog.txt @end example @noindent The parameters of the mock profiles can either be given through a catalog (which stores the parameters of many mock profiles, see @ref{MakeProfiles catalog}), or the @option{--kernel} option (see @ref{MakeProfiles output dataset}). The catalog can be in the FITS ASCII, FITS binary format, or plain text formats (see @ref{Tables}). The columns related to each parameter can be determined both by number, or by match/search criteria using the column names, units, or comments. with the options ending in @option{col}, see below. Without any file given to the @option{--background} option, MakeProfiles will make a zero-valued image and build the profiles on that (its size and main WCS parameters can also be defined through the options described in @ref{MakeProfiles output dataset}). Besides the main/merged image containing all the profiles in the catalog, it is also possible to build individual images for each profile (only enclosing one full profile to its truncation radius) with the @option{--individual} option. If an image is given to the @option{--background} option, the pixels of that image are used as the background value for every pixel. The flux value of each profile pixel will be added to the pixel in that background value. In this case, the values to all options relating to the output size and WCS will be ignored if specified (for example @option{--oversample}, @option{--naxis}, and @option{--prepforconv}) on the command-line or in the configuration files. The sections below discuss the options specific to MakeProfiles based on context: the input catalog settings which can have many rows for different profiles are discussed in @ref{MakeProfiles catalog}, in @ref{MakeProfiles profile settings}, we discuss how you can set general profile settings (that are the same for all the profiles in the catalog). Finally @ref{MakeProfiles output dataset} and @ref{MakeProfiles log file} discuss the outputs of MakeProfiles and how you can configure them. Besides these, MakeProfiles also supports all the common Gnuastro program options that are discussed in @ref{Common options}, so please flip through them is well for a more comfortable usage. Please see @ref{Sufi simulates a detection} for a very complete tutorial explaining how one could use MakeProfiles in conjunction with other Gnuastro's programs to make a complete simulated image of a mock galaxy. @menu * MakeProfiles catalog:: Required catalog properties. * MakeProfiles profile settings:: Configuration parameters for all profiles. * MakeProfiles output dataset:: The canvas/dataset to build profiles over. * MakeProfiles log file:: A description of the optional log file. @end menu @node MakeProfiles catalog, MakeProfiles profile settings, Invoking astmkprof, Invoking astmkprof @subsubsection MakeProfiles catalog The catalog containing information about each profile can be in the FITS ASCII, FITS binary, or plain text formats (see @ref{Tables}). Its columns can be ordered in any desired manner. You can specify which columns belong to which parameters using the set of options discussed below. For example through the @option{--rcol} and @option{--tcol} options, you can specify the column that contains the radial parameter for each profile and its truncation respectively. See @ref{Selecting table columns} for a thorough discussion on the values to these options. The value for the profile center in the catalog (the @option{--ccol} option) can be a floating point number so the profile center can be on any sub-pixel position. Note that pixel positions in the FITS standard start from 1 and an integer is the pixel center. So a 2D image actually starts from the position (0.5, 0.5), which is the bottom-left corner of the first pixel. When a @option{--background} image with WCS information is provided or you specify the WCS parameters with the respective options, you may also use RA and Dec to identify the center of each profile (see the @option{--mode} option below). In MakeProfiles, profile centers do not have to be in (overlap with) the final image. Even if only one pixel of the profile within the truncation radius overlaps with the final image size, the profile is built and included in the final image image. Profiles that are completely out of the image will not be created (unless you explicity ask for it with the @option{--individual} option). You can use the output log file (created with @option{--log} to see which profiles were within the image, see @ref{Common options}. If PSF profiles (Moffat or Gaussian, see @ref{PSF}) are in the catalog and the profiles are to be built in one image (when @option{--individual} is not used), it is assumed they are the PSF(s) you want to convolve your created image with. So by default, they will not be built in the output image but as separate files. The sum of pixels of these separate files will also be set to unity (1) so you are ready to convolve, see @ref{Convolution process}. As a summary, the position and magnitude of PSF profile will be ignored. This behavior can be disabled with the @option{--psfinimg} option. If you want to create all the profiles separately (with @option{--individual}) and you want the sum of the PSF profile pixels to be unity, you have to set their magnitudes in the catalog to the zero-point magnitude and be sure that the central positions of the profiles don't have any fractional part (the PSF center has to be in the center of the pixel). The list of options directly related to the input catalog columns is shown below. @table @option @item --ccol=STR/INT Center coordinate column for each dimension. This option must be called two times to define the center coordinates in an image. For example @option{--ccol=RA} and @option{--ccol=DEC} (along with @option{--mode=wcs}) will inform MakeProfiles to look into the catalog columns named @option{RA} and @option{DEC} for the Right Ascension and Declination of the profile centers. @item --fcol=INT/STR The functional form of the profile with one of the values below depending on the desired profile. The column can contain either the numeric codes (for example `@code{1}') or string characters (for example `@code{sersic}'). The numeric codes are easier to use in scripts which generate catalogs with hundreds or thousands of profiles. The string format can be easier when the catalog is to be written/checked by hand/eye before running MakeProfiles. It is much more readable and provides a level of documentation. All Gnuastro's recognized table formats (see @ref{Recognized table formats}) accept string type columns. To have string columns in a plain text table/catalog, see @ref{Gnuastro text table format}. @itemize @item S@'ersic profile with `@code{sersic}' or `@code{1}'. @item Moffat profile with `@code{moffat}' or `@code{2}'. @item Gaussian profile with `@code{gaussian}' or `@code{3}'. @item Point source with `@code{point}' or `@code{4}'. @item Flat profile with `@code{flat}' or `@code{5}'. @item Circumference profile with `@code{circum}' or `@code{6}'. A fixed value will be used for all pixels between the truncation radius (@mymath{r_t}) and @mymath{r_t-w} (@mymath{w} is the value to the @option{--circumwidth}). @item Radial distance profile with `@code{distance}' or `@code{7}'. At the lowest level, each pixel only has an elliptical radial distance given the profile's shape and orentiation (see @ref{Defining an ellipse}). When this profile is chosen, the pixel's elliptical radial distance from the profile center is written as its value. For this profile, the value in the magnitude column (@option{--mcol}) will be ignored. You can use this for checks or as a first approximation to define your own higher-level radial function. In the latter case, just note that the central values are going to be incorrect (see @ref{Sampling from a function}). @end itemize @item --rcol=STR/INT The radius parameter of the profiles. Effective radius (@mymath{r_e}) if S@'ersic, FWHM if Moffat or Gaussian. @item --ncol=STR/INT The S@'ersic index (@mymath{n}) or Moffat @mymath{\beta}. @item --pcol=STR/INT The position angle (in degrees) of the profiles relative to the first FITS axis (horizontal when viewed in SAO ds9). @item --qcol=STR/INT The axis ratio of the profiles (minor axis divided by the major axis in a 2D ellipse). @item --mcol=STR/INT The total pixelated magnitude of the profile within the truncation radius, see @ref{Profile magnitude}. @item --tcol=STR/INT The truncation radius of this profile. By default it is in units of the radial parameter of the profile (the value in the @option{--rcol} of the catalog). If @option{--tunitinp} is given, this value is interpreted in units of pixels (prior to oversampling) irrespective of the profile. @end table @node MakeProfiles profile settings, MakeProfiles output dataset, MakeProfiles catalog, Invoking astmkprof @subsubsection MakeProfiles profile settings The profile parameters that differ between each created profile are specified through the columns in the input catalog and described in @ref{MakeProfiles catalog}. Besides those there are general settings for some profiles that don't differ between one profile and another, they are a property of the general process. For example how many random points to use in the monte-carlo integration, this value is fixed for all the profiles. The options described in this section are for configuring such properties. @table @option @item --mode=STR Interpret the center position columns (@option{--ccol} in @ref{MakeProfiles catalog}) in image or WCS coordinates. This option thus accepts only two values: @option{img} and @option{wcs}. It is mandatory when a catalog is being used as input. @item -r @itemx --numrandom The number of random points used in the central regions of the profile, see @ref{Sampling from a function}. @item -e @itemx --envseed Use the value to the @code{GSL_RNG_SEED} environment variable to generate the random Monte Carlo sampling distribution, see @ref{Sampling from a function} and @ref{Generating random numbers}. @item -t FLT @itemx --tolerance=FLT The tolerance to switch from Monte Carlo integration to the central pixel value, see @ref{Sampling from a function}. @item -p @itemx --tunitinp The truncation column of the catalog is in units of pixels. By default, the truncation column is considered to be in units of the radial parameters of the profile (@option{--rcol}). Read it as `t-unit-in-p' for `truncation unit in pixels'. @item -f @itemx --mforflatpix When making fixed value profiles (flat and circumference, see `@option{--fcol}'), don't use the value in the column specified by `@option{--mcol}' as the magnitude. Instead use it as the exact value that all the pixels of these profiles should have. This option is irrelevant for other types of profiles. This option is very useful for creating masks, or labeled regions in an image. Any integer, or floating point value can used in this column with this option, including @code{NaN} (or `@code{nan}', or `@code{NAN}', case is irrelevant), and infinities (@code{inf}, @code{-inf}, or @code{+inf}). For example, with this option if you set the value in the magnitude column (@option{--mcol}) to @code{NaN}, you can create an elliptical or circular mask over an image (which can be given as the argument), see @ref{Blank pixels}. Another useful application of this option is to create labeled elliptical or circular apertures in an image. To do this, set the value in the magnitude column to the label you want for this profile. This labeled image can then be used in combination with NoiseChisel's output (see @ref{NoiseChisel output}) to do aperture photometry with MakeCatalog (see @ref{MakeCatalog}). Alternatively, if you want to mark regions of the image (for example with an elliptical circumference) and you don't want to use NaN values (as explained above) for some technical reason, you can get the minimum or maximum value in the image @footnote{The minimum will give a better result, because the maximum can be too high compared to most pixels in the image, making it harder to display.} using Arithmetic (see @ref{Arithmetic}), then use that value in the magnitude column along with this option for all the profiles. Please note that when using MakeProfiles on an already existing image, you have to set `@option{--oversample=1}'. Otherwise all the profiles will be scaled up based on the oversampling scale in your configuration files (see @ref{Configuration files}) unless you have accounted for oversampling in your catalog. @item --mcolisbrightness The value given in the ``magnitude column'' (specified by @option{--mcol}, see @ref{MakeProfiles catalog}) must be interpretted as brightness, not magnitude. The zeropoint magnitude (value to the @option{--zeropoint} option) is ignored and the given value must have the same units as the input dataset's pixels. Recall that the total profile magnitude or brightness that is specified with in the @option{--mcol} column of the input catalog is not an integration to infinity, but the actual sum of pixels in the profile (until the desired truncation radius). See @ref{Profile magnitude} for more on this point. @item --magatpeak The magnitude column in the catalog (see @ref{MakeProfiles catalog}) will be used to find the brightness only for the peak profile pixel, not the full profile. Note that this is the flux of the profile's peak pixel in the final output of MakeProfiles. So beware of the oversampling, see @ref{Oversampling}. This option can be useful if you want to check a mock profile's total magnitude at various truncation radii. Without this option, no matter what the truncation radius is, the total magnitude will be the same as that given in the catalog. But with this option, the total magnitude will become brighter as you increase the truncation radius. In sharper profiles, sometimes the accuracy of measuring the peak profile flux is more than the overall object brightness. In such cases, with this option, the final profile will be built such that its peak has the given magnitude, not the total profile. @cartouche @strong{CAUTION:} If you want to use this option for comparing with observations, please note that MakeProfiles does not do convolution. Unless you have de-convolved your data, your images are convolved with the instrument and atmospheric PSF, see @ref{PSF}. Particularly in sharper profiles, the flux in the peak pixel is strongly decreased after convolution. Also note that in such cases, besides de-convolution, you will have to set @option{--oversample=1} otherwise after resampling your profile with Warp (see @ref{Warp}), the peak flux will be different. @end cartouche @item -X INT,INT @itemx --shift=INT,INT Shift all the profiles and enlarge the image along each dimension. To better understand this option, please see @mymath{n} in @ref{If convolving afterwards}. This is useful when you want to convolve the image afterwards. If you are using an external PSF, be sure to oversample it to the same scale used for creating the mock images. If a background image is specified, any possible value to this option is ignored. @item -c @itemx --prepforconv Shift all the profiles and enlarge the image based on half the width of the first Moffat or Gaussian profile in the catalog, considering any possible oversampling see @ref{If convolving afterwards}. @option{--prepforconv} is only checked and possibly activated if @option{--xshift} and @option{--yshift} are both zero (after reading the command-line and configuration files). If a background image is specified, any possible value to this option is ignored. @item -z FLT @itemx --zeropoint=FLT The zero-point magnitude of the image. @item -w FLT @itemx --circumwidth=FLT The width of the circumference if the profile is to be an elliptical circumference or annulus. See the explanations for this type of profile in @option{--fcol}. @item -R @itemx --replace Do not add the pixels of each profile over the background (possibly crowded by other profiles), replace them. By default, when two profiles overlap, the final pixel value is the sum of all the profiles that overlap on that pixel. When this option is given, the pixels are not added but replaced by the newer profile's pixel and any value under it is lost. @cindex CPU threads @cindex Threads, CPU When order matters, make sure to use this function with `@option{--numthreads=1}'. When multiple threads are used, the separate profiles are built asynchronously and not in order. Since order does not matter in an addition, this causes no problems by default but has to be considered when this option is given. Using multiple threads is no problem if the profiles are to be used as a mask with a blank or fixed value (see `@option{--mforflatpix}') since all their pixel values are the same. Note that only non-zero pixels are replaced. With radial profiles (for example S@'ersic or Moffat) only values above zero will be part of the profile. However, when using flat profiles with the `@option{--mforflatpix}' option, you should be careful not to give a @code{0.0} value as the flat profile's pixel value. @end table @node MakeProfiles output dataset, MakeProfiles log file, MakeProfiles profile settings, Invoking astmkprof @subsubsection MakeProfiles output dataset MakeProfiles takes an input catalog uses basic properties that are defined there to build a dataset, for example a 2D image containing the profiles in the catalog. In @ref{MakeProfiles catalog} and @ref{MakeProfiles profile settings}, the catalog and profile settings were discussed. The options of this section, allow you to configure the output dataset (or the canvas that will host the built profiles). @table @option @item -k STR @itemx --background=STR A background image FITS file to build the profiles on. The extension that contains the image should be specified with the @option{--backhdu} option, see below. When a background image is specified, it will be used to derive all the information about the output image. Hence, the following options will be ignored: @option{--naxis}, @option{--oversample}, @option{--crpix}, @option{--crval} (generally, all other WCS related parameters) and the output's data type (see @option{--type} in @ref{Input output options}). The image will act like a canvas to build the profiles on: profile pixel values will be summed with the background image pixel values. With the @option{--replace} option you can disable this behavior and replace the profile pixels with the background pixels. If you want to use all the image information above, except for the pixel values (you want to have a blank canvas to build the profiles on, based on an input image), you can call @option{--clearcanvas}, to set all the input image's pixels to zero before starting to build the profiles over it (this is done in memory after reading the input, so nothing will happen to your input file). @item -B STR/INT @itemx --backhdu=STR/INT The header data unit (HDU) of the file given to @option{--background}. @item -C @itemx --clearcanvas When an input image is specified (with the @option{--background} option, set all its pixels to 0.0 immediately after reading it into memory. Effectively, this will allow you to use all its properties (described under the @option{--background} option), without having to worry about the pixel values. @option{--clearcanvas} can come in handy in many situations, for example if you want to create a labeled image (segmentation map) for creating a catalog (see @ref{MakeCatalog}). In other cases, you might have modeled the objects in an image and want to create them on the same frame, but without the original pixel values. @item -E STR/INT,FLT[,FLT,[...]] @itemx --kernel=STR/INT,FLT[,FLT,[...]] Only build one kernel profile with the parameters given as the values to this option. The different values must be separated by a comma (@key{,}). The first value identifies the radial function of the profile, either through a string or through a number (see description of @option{--fcol} in @ref{MakeProfiles catalog}). Each radial profile needs a different total number of parameters: S@'ersic and Moffat functions need 3 parameters: radial, S@'ersic index or Moffat @mymath{\beta}, and truncation radius. The Gaussian function needs two parameters: radial and truncation radius. The point function doesn't need any parameters and flat and circumference profiles just need one parameter (truncation radius). The PSF or kernel is a unique (and highly constrained) type of profile: the sum of its pixels must be one, its center must be the center of the central pixel (in an image with an odd number of pixels on each side), and commonly it is circular, so its axis ratio and position angle are one and zero respectively. Kernels are commonly necessary for various data analysis and data manipulation steps (for example see @ref{Convolve}, and @ref{NoiseChisel}. Because of this it is inconvenient to define a catalog with one row and many zero valued columns (for all the non-necessary parameters). Hence, with this option, it is possible to create a kernel with MakeProfiles without the need to create a catalog. Here are some examples: @table @option @item --kernel=moffat,3,2.8,5 A Moffat kernel with FWHM of 3 pixels, @mymath{\beta=2.8} which is truncated at 5 times the FWHM. @item --kernel=gaussian,2,3 A Gaussian kernel with FWHM of 2 pixels and truncated at 3 times the FWHM. @end table @item -x INT,INT @itemx --naxis=INT,INT The number of pixels along each dimension axis of the output in FITS order. This is before over-sampling. For example if you call MakeProfiles with @option{--naxis=100,150 --oversample=5} (assuming no shift due for later convolution), then the final image size along the first axis will be 500 by 750 pixels. Fractions are acceptable as values for each dimension, however, they must reduce to an integer, so @option{--naxis=150/3,300/3} is acceptable but @option{--naxis=150/4,300/4} is not. When viewing a FITS image in DS9, the first FITS dimension is in the horizontal direction and the second is vertical. As an example, the image created with the example above will have 500 pixels horizontally and 750 pixels vertically. If a background image is specified, this option is ignored. @item -s INT @itemx --oversample=INT The scale to over-sample the profiles and final image. If not an odd number, will be added by one, see @ref{Oversampling}. Note that this @option{--oversample} will remain active even if an input image is specified. If your input catalog is based on the background image, be sure to set @option{--oversample=1}. @item --psfinimg Build the possibly existing PSF profiles (Moffat or Gaussian) in the catalog into the final image. By default they are built separately so you can convolve your images with them, thus their magnitude and positions are ignored. With this option, they will be built in the final image like every other galaxy profile. To have a final PSF in your image, make a point profile where you want the PSF and after convolution it will be the PSF. @item -i @itemx --individual @cindex Individual profiles @cindex Build individual profiles If this option is called, each profile is created in a separate FITS file within the same directory as the output and the row number of the profile (starting from zero) in the name. The file for each row's profile will be in the same directory as the final combined image of all the profiles and will have the final image's name as a suffix. So for example if the final combined image is named @file{./out/fromcatalog.fits}, then the first profile that will be created with this option will be named @file{./out/0_fromcatalog.fits}. Since each image only has one full profile out to the truncation radius the profile is centered and so, only the sub-pixel position of the profile center is important for the outputs of this option. The output will have an odd number of pixels. If there is no oversampling, the central pixel will contain the profile center. If the value to @option{--oversample} is larger than unity, then the profile center is on any of the central @option{--oversample}'d pixels depending on the fractional value of the profile center. If the fractional value is larger than half, it is on the bottom half of the central region. This is due to the FITS definition of a real number position: The center of a pixel has fractional value @mymath{0.00} so each pixel contains these fractions: .5 -- .75 -- .00 (pixel center) -- .25 -- .5. @item -m @itemx --nomerged Don't make a merged image. By default after making the profiles, they are added to a final image with side lengths specified by @option{--naxis}if they overlap with it. @end table @noindent The options below can be used to define the world coordinate system (WCS) properties of the MakeProfiles outputs. The option names are delibarately chosen to be the same as the FITS standard WCS keywords. See Section 8 of @url{https://doi.org/10.1051/0004-6361/201015362, Pence et al [2010]} for a short introduction to WCS in the FITS standard@footnote{The world coordinate standard in FITS is a very beatiful and powerful concept to link/associate datasets with the outside world (other datasets). The description in the FITS standard (link above) only touches the tip of the ice-burg. To learn more please see @url{https://doi.org/10.1051/0004-6361:20021326, Greisen and Calabretta [2002]}, @url{https://doi.org/10.1051/0004-6361:20021327, Calabretta and Greisen [2002]}, @url{https://doi.org/10.1051/0004-6361:20053818, Greisen et al. [2006]}, and @url{http://www.atnf.csiro.au/people/mcalabre/WCS/dcs_20040422.pdf, Calabretta et al.}}. If you look into the headers of a FITS image with WCS for example you will see all these names but in uppercase and with numbers to represent the dimensions, for example @code{CRPIX1} and @code{PC2_1}. You can see the FITS headers with Gnuastro's @ref{Fits} program using a command like this: @command{$ astfits -p image.fits}. If the values given to any of these options does not correspond to the number of dimensions in the output dataset, then no WCS information will be added. @table @option @item --crpix=FLT,FLT The pixel coordinates of the WCS reference point. Fractions are acceptable for the values of this option. @item --crval=FLT,FLT The WCS coordinates of the Reference point. Fractions are acceptable for the values of this option. @item --cdelt=FLT,FLT The resolution (size of one data-unit or pixel in WCS units) of the non-oversampled dataset. Fractions are acceptable for the values of this option. @item --pc=FLT,FLT,FLT,FLT The PC matrix of the WCS rotation, see the FITS standard (link above) to better understand the PC matrix. @item --cunit=STR,STR The units of each WCS axis, for example @code{deg}. Note that these values are part of the FITS standard (link above). MakeProfiles won't complain if you use non-standard values, but later usage of them might cause trouble. @item --ctype=STR,STR The type of each WCS axis, for example @code{RA---TAN} and @code{DEC--TAN}. Note that these values are part of the FITS standard (link above). MakeProfiles won't complain if you use non-standard values, but later usage of them might cause trouble. @end table @node MakeProfiles log file, , MakeProfiles output dataset, Invoking astmkprof @subsubsection MakeProfiles log file Besides the final merged dataset of all the profiles, or the individual datasets (see @ref{MakeProfiles output dataset}), if the @option{--log} option is called MakeProfiles will also create a log file in the current directory (where you run MockProfiles). See @ref{Common options} for a full description of @option{--log} and other options that are shared between all Gnuastro programs. The values for each column are explained in the first few commented lines of the log file (starting with @command{#} character). Here is a more complete description. @itemize @item An ID (row number of profile in input catalog). @item The total magnitude of the profile in the output dataset. When the profile does not completely overlap with the output dataset, this will be different from your input magnitude. @item The number of pixels (in the oversampled image) which used Monte Carlo integration and not the central pixel value, see @ref{Sampling from a function}. @item The fraction of flux in the Monte Carlo integrated pixels. @item If an individual image was created, this column will have a value of @code{1}, otherwise it will have a value of @code{0}. @end itemize @node MakeNoise, , MakeProfiles, Modeling and fittings @section MakeNoise @cindex Noise Real data are always buried in noise, therefore to finalize a simulation of real data (for example to test our observational algorithms) it is essential to add noise to the mock profiles created with MakeProfiles, see @ref{MakeProfiles}. Below, the general principles and concepts to help understand how noise is quantified is discussed. MakeNoise options and argument are then discussed in @ref{Invoking astmknoise}. @menu * Noise basics:: Noise concepts and definitions. * Invoking astmknoise:: Options and arguments to MakeNoise. @end menu @node Noise basics, Invoking astmknoise, MakeNoise, MakeNoise @subsection Noise basics @cindex Noise @cindex Image noise Deep astronomical images, like those used in extragalactic studies seriously suffer from noise in the data. Generally speaking, the sources of noise in an astronomical image are photon counting noise and Instrumental noise which are discussed in detail below. We finish with a short introduction on how random numbers are generated and how you can determine the random number generator and seed value. @menu * Photon counting noise:: Poisson noise * Instrumental noise:: Readout, dark current and other sources. * Final noised pixel value:: How the final noised value is calculated. * Generating random numbers:: How random numbers are generated. @end menu @node Photon counting noise, Instrumental noise, Noise basics, Noise basics @subsubsection Photon counting noise @cindex Counting error @cindex Photon counting noise Thanks to the very accurate electronics used in today's detectors, this type of noise is the main cause of concern for extra galactic studies. It can generally be associate with the counting error that is known to have a Poisson distribution. The Poisson distribution is about counting. But counting is a discrete operation with only positive values, for example we can't count @mymath{3.2} or @mymath{-2} of anything. We only count @mymath{0}, @mymath{1}, @mymath{2}, @mymath{3} and so on. Therefore the Poisson distribution is also a discrete distribution, only applying to whole positive integers. @cindex Probability density function Let's assume the mean value of counting something is known. In this case, we are counting the number of electrons that are produced by photons in a detector (for example CCD) pixel. Let's call this mean @mymath{\lambda}. Furthermore, let's take @mymath{k} to represent the result of one particular counting attempt. The probability density function of @mymath{k} can be written as: @cindex Poisson distribution @dispmath{f(k)={\lambda^k \over k!} e^{-\lambda},\quad k\in @{0, 1, 2, 3, \dots @}} @cindex Skewed Poisson distribution Because the Poisson distribution is only applicable to positive values, naturally it is very skewed when @mymath{\lambda} is near zero. One qualitative way to explain it is that there simply aren't enough integers smaller than @mymath{\lambda}, than integers that are larger than it. Therefore to accommodate all possibilities, it has to be skewed when @mymath{\lambda} is small. @cindex Compare Poisson and Gaussian But as @mymath{\lambda} becomes larger and larger, the distribution becomes more and more symmetric. One very useful property of the Poisson distribution is that the mean value is also its variance. When @mymath{\lambda} is very large, say @mymath{\lambda>1000}, then the normal (Gaussian) distribution, see @ref{PSF}, is an excellent approximation of the Poisson distribution with mean @mymath{\mu=\lambda} and standard deviation @mymath{\sigma=\sqrt{\lambda}}. We see that the variance or dispersion of the distribution depends on the mean value, and when it is large it can be approximated with a Gaussian that only has one free parameter (@mymath{\mu=\lambda} and @mymath{\sigma=\sqrt{\lambda}}) instead of two that it originally has. @cindex Sky value @cindex Background flux @cindex Undetected objects The astronomical objects after convolution with the PSF of the instrument, lie above a certain background flux. This background flux is defined to be the average flux of a region in the image that has absolutely no objects. The physical origin of this background value is the brightness of the atmosphere or possible stray light within the imaging instrument. It is thus an ideal definition, because in practice, what lies deep in the noise far lower than the detection limit is never known@footnote{See the section on sky in Akhlaghi M., Ichikawa. T. 2015. Astrophysical Journal Supplement Series.}. However, in a real image, a relatively large number of very faint objects can been fully buried in the noise. These undetected objects will bias the background measurement to slightly larger values. The sky value is therefore defined to be the average of the undetected regions in the image, so in an ideal case where all the objects have been detected, the sky value and background value are the same. @cindex Background flux gradients @cindex Gradients in background flux @cindex Variation of background flux As longer wavelengths are used, the background value becomes more significant and also varies over a wide image field. Such variations are not currently implemented in MakeProfiles, but will be in the future. In a mock image, we have the luxury of setting the background value. @cindex Simulating noise @cindex Noise simulation In each pixel of the canvas of pixels, the flux is the sum of contributions from various sources after convolution. Let's name this flux of the convolved sum of possibly overlapping objects, @mymath{I_{nn}}. @mymath{nn} representing `no noise'. For now, let's assume the background is constant and represented by @mymath{B}. In practice the background values are larger than @mymath{\sim1,000} counts. Then the flux after adding noise is a random value taken from a Gaussian distribution with the following mean (@mymath{\mu}) and standard deviation (@mymath{\sigma}): @dispmath{\mu=B+I_{nn}, \quad \sigma=\sqrt{B+I_{nn}}} Since this type of noise is inherent in the objects we study, it is usually measured on the same scale as the astronomical objects, namely the magnitude system, see @ref{Flux Brightness and magnitude}. It is then internally converted to the flux scale for further processing. @node Instrumental noise, Final noised pixel value, Photon counting noise, Noise basics @subsubsection Instrumental noise @cindex Readout noise @cindex Instrumental noise @cindex Noise, instrumental While taking images with a camera, a dark current is fed to the pixels, the variation of the value of this dark current over the pixels, also adds to the final image noise. Another source of noise is the readout noise that is produced by the electronics in the CCD that attempt to digitize the voltage produced by the photo-electrons in the analog to digital converter. In deep extra-galactic studies these sources of noise are not as significant as the noise of the background sky. Let @mymath{C} represent the combined standard deviation of all these sources of noise. If only this source of noise is present, the noised pixel value would be a random value chosen from a Gaussian distribution with @dispmath{\mu=I_{nn}, \quad \sigma=\sqrt{C^2+I_{nn}}} @cindex ADU @cindex Gain @cindex Counts This type of noise is completely independent of the type of objects being studied, it is completely determined by the instrument. So the flux scale (and not magnitude scale) is most commonly used for this type of noise. In practice, this value is usually reported in ADUs not flux or electron counts. The gain value of the device can be used to convert between these two, see @ref{Flux Brightness and magnitude}. @node Final noised pixel value, Generating random numbers, Instrumental noise, Noise basics @subsubsection Final noised pixel value Depending on the values you specify for @mymath{B} and @mymath{C} from the above, the final noised value for each pixel is a random value chosen from a Gaussian distribution with @dispmath{\mu=B+I_{nn}, \quad \sigma=\sqrt{C^2+B+I_{nn}}} @node Generating random numbers, , Final noised pixel value, Noise basics @subsubsection Generating random numbers @cindex Random numbers @cindex Numbers, random As discussed above, to generate noise we need to make random samples of a particular distribution. So it is important to understand some general concepts regarding the generation of random numbers. For a very complete and nice introduction we strongly advise reading Donald Knuth's ``The art of computer programming'', volume 2, chapter 3@footnote{Knuth, Donald. 1998. The art of computer programming. Addison--Wesley. ISBN 0-201-89684-2 }. Quoting from the GNU Scientific Library manual, ``If you don't own it, you should stop reading right now, run to the nearest bookstore, and buy it''@footnote{For students, running to the library might be more affordable!}! @cindex Psudo-random numbers @cindex Numbers, psudo-random @cindex Seed, psudo-random numbers Using only software, we can only produce what is called a psudo-random sequence of numbers. A true random number generator is a hardware (let's assume we have made sure it has no systematic biases), for example throwing dice or flipping coins (which have remained from the ancient times). More modern hardware methods use atmospheric noise, thermal noise or other types of external electromagnetic or quantum phenomena. All psudo-random number generators (software) require a seed to be the basis of the generation. The advantage of having a seed is that if you specify the same seed for multiple runs, you will get an identical sequence of random numbers which allows you to reproduce the same final noised image. @cindex Environment variables @cindex GNU Scientific Library The programs in GNU Astronomy Utilities (for example MakeNoise or MakeProfiles) use the GNU Scientific Library (GSL) to generate random numbers. GSL allows the user to set the random number generator through environment variables, see @ref{Installation directory} for an introduction to environment variables. In the chapter titled ``Random Number Generation'' they have fully explained the various random number generators that are available (there are a lot of them!). Through the two environment variables @code{GSL_RNG_TYPE} and @code{GSL_RNG_SEED} you can specify the generator and its seed respectively. If you don't specify a value for @code{GSL_RNG_TYPE}, GSL will use its default random number generator type. The default type is sufficient for most general applications. If no value is given for the @code{GSL_RNG_SEED} environment variable and you have asked Gnuastro to read the seed from the environment (through the @option{--envseed} option), then GSL will use the default value of each generator to give identical outputs. If you don't explicitly tell Gnuastro programs to read the seed value from the environment variable, then they will use the system time (accurate to within a microsecond) to generate (apparently random) seeds. In this manner, every time you run the program, you will get a different random number distribution. There are two ways you can specify values for these environment variables. You can call them on the same command-line for example: @example $ GSL_RNG_TYPE="taus" GSL_RNG_SEED=345 astmknoise input.fits @end example @noindent In this manner the values will only be used for this particular execution of MakeNoise. Alternatively, you can define them for the full period of your terminal session or script length, using the shell's @command{export} command with the two separate commands below (for a script remove the @code{$} signs): @example $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 @end example @cindex Startup scripts @cindex @file{.bashrc} @noindent The subsequent programs which use GSL's random number generators will hence forth use these values in this session of the terminal you are running or while executing this script. In case you want to set fixed values for these parameters every time you use the GSL random number generator, you can add these two lines to your @file{.bashrc} startup script@footnote{Don't forget that if you are going to give your scripts (that use the GSL random number generator) to others you have to make sure you also tell them to set these environment variable separately. So for scripts, it is best to keep all such variable definitions within the script, even if they are within your @file{.bashrc}.}, see @ref{Installation directory}. @cartouche @noindent @strong{NOTE:} If the two environment variables @code{GSL_RNG_TYPE} and @code{GSL_RNG_SEED} are defined, GSL will report them by default, even if you don't use the @option{--envseed} option. For example you can see the top few lines of the output of MakeProfiles: @example $ export GSL_RNG_TYPE="taus" $ export GSL_RNG_SEED=345 $ astmkprof catalog.txt --envseed GSL_RNG_TYPE=taus GSL_RNG_SEED=345 MakeProfiles started on AAA BBB DD EE:FF:GG HHH - 6 profiles read from catalog.txt 0.000236 seconds - Random number generator (RNG) type: taus - RNG seed for all profiles: 345 @end example @noindent The first two output lines (showing the names of the environment variables) are printed by GSL before MakeProfiles actually starts generating random numbers. The Gnuastro programs will report the values they use independently, you should check them for the final values used. For example if @option{--envseed} is not given, @code{GSL_RNG_SEED} will not be used and the last line shown above will not be printed. In the case of MakeProfiles, each profile will get its own seed value. @end cartouche @node Invoking astmknoise, , Noise basics, MakeNoise @subsection Invoking MakeNoise MakeNoise will add noise to an existing image. The executable name is @file{astmknoise} with the following general template @example $ astmknoise [OPTION ...] InputImage.fits @end example @noindent One line examples: @example ## Add noise with a standard deviation of 100 to image: $ astmknoise --sigma=100 image.fits ## Add noise to input image assuming a background magnitude (with ## zeropoint magnitude of 0) and a certain instrumental noise: $ astmknoise --background=-10 -z0 --instrumental=20 mockimage.fits @end example @noindent If actual processing is to be done, the input image is a mandatory argument. The full list of options common to all the programs in Gnuastro can be seen in @ref{Common options}. The type (see @ref{Numeric data types}) of the output can be specified with the @option{--type} option, see @ref{Input output options}. The header of the output FITS file keeps all the parameters that were influential in making it. This is done for future reproducibility. @table @option @item -s FLT @item --sigma=FLT The total noise sigma in the same units as the pixel values. With this option, the @option{--background}, @option{--zeropoint} and @option{--instrumental} will be ignored. With this option, the noise will be independent of the pixel values (which is not realistic, see @ref{Photon counting noise}). Hence it is only useful if you are working on low surface brightness regions where the change in pixel value (and thus real noise) is insignificant. @item -b FLT @itemx --background=FLT The background pixel value for the image in units of magnitudes, see @ref{Photon counting noise} and @ref{Flux Brightness and magnitude}. @item -z FLT @itemx --zeropoint=FLT The zeropoint magnitude used to convert the value of @option{--background} (in units of magnitude) to flux, see @ref{Flux Brightness and magnitude}. @item -i FLT @itemx --instrumental=FLT The instrumental noise which is in units of flux, see @ref{Instrumental noise}. @item -e @itemx --envseed Use the @code{GSL_RNG_SEED} environment variable for the seed used in the random number generator, see @ref{Generating random numbers}. With this option, the output image noise is always going to be identical (or reproducible). @item -d @itemx --doubletype Save the output in the double precision floating point format that was used internally. This option will be most useful if the input images were of integer types. @end table @node High-level calculations, Library, Modeling and fittings, Top @chapter High-level calculations After the reduction of raw data (for example with the programs in @ref{Data manipulation}) you will have reduced images/data ready for processing/analyzing (for example with the programs in @ref{Data analysis}). But the processed/analyzed data (or catalogs) are still not enough to derive any scientific result. Even higher-level analysis is still needed to convert the observed magnitudes, sizes or volumes into physical quantities that we associate with each catalog entry or detected object which is the purpose of the tools in this section. @menu * CosmicCalculator:: Calculate cosmological variables @end menu @node CosmicCalculator, , High-level calculations, High-level calculations @section CosmicCalculator To derive higher-level information regarding our sources in extra-galactic astronomy, cosmological calculations are necessary. In Gnuastro, CosmicCalculator is in charge of such calculations. Before discussing how CosmicCalculator is called and operates (in @ref{Invoking astcosmiccal}), it is important to provide a rough but mostly self sufficient review of the basics and the equations used in the analysis. In @ref{Distance on a 2D curved space} the basic idea of understanding distances in a curved and expanding 2D universe (which we can visualize) are reviewed. Having solidified the concepts there, in @ref{Extending distance concepts to 3D}, the formalism is extended to the 3D universe we are trying to study in our research. The focus here is obtaining a physical insight into these equations (mainly for the use in real observational studies). There are many books thoroughly deriving and proving all the equations with all possible initial conditions and assumptions for any abstract universe, interested readers can study those books. @menu * Distance on a 2D curved space:: Distances in 2D for simplicity * Extending distance concepts to 3D:: Going to 3D (our real universe). * Invoking astcosmiccal:: How to run CosmicCalculator @end menu @node Distance on a 2D curved space, Extending distance concepts to 3D, CosmicCalculator, CosmicCalculator @subsection Distance on a 2D curved space The observations to date (for example the Planck 2015 results), have not measured@footnote{The observations are interpreted under the assumption of uniform curvature. For a relativistic alternative to dark energy (and maybe also some part of dark matter), non-uniform curvature may be even be more critical, but that is beyond the scope of this brief explanation.} the presence of significant curvature in the universe. However to be generic (and allow its measurement if it does in fact exist), it is very important to create a framework that allows non-zero uniform curvature. However, this section is not intended to be a fully thorough and mathematically complete derivation of these concepts. There are many references available for such reviews that go deep into the abstract mathematical proofs. The emphasis here is on visualization of the concepts for a beginner. As 3D beings, it is difficult for us to mentally create (visualize) a picture of the curvature of a 3D volume. Hence, here we will assume a 2D surface/space and discuss distances on that 2D surface when it is flat and when it is curved. Once the concepts have been created/visualized here, we will extend them, in @ref{Extending distance concepts to 3D}, to a real 3D spatial @emph{slice} of the Universe we live in and hope to study. To be more understandable (actively discuss from an observer's point of view) let's assume there's an imaginary 2D creature living on the 2D space (which @emph{might} be curved in 3D). Here, we will be working with this creature in its efforts to analyze distances in its 2D universe. The start of the analysis might seem too mundane, but since it is difficult to imagine a 3D curved space, it is important to review all the very basic concepts thoroughly for an easy transition to a universe that is more difficult to visualize (a curved 3D space embedded in 4D). To start, let's assume a static (not expanding or shrinking), flat 2D surface similar to @ref{flatplane} and that the 2D creature is observing its universe from point @mymath{A}. One of the most basic ways to parametrize this space is through the Cartesian coordinates (@mymath{x}, @mymath{y}). In @ref{flatplane}, the basic axes of these two coordinates are plotted. An infinitesimal change in the direction of each axis is written as @mymath{dx} and @mymath{dy}. For each point, the infinitesimal changes are parallel with the respective axes and are not shown for clarity. Another very useful way of parameterizing this space is through polar coordinates. For each point, we define a radius (@mymath{r}) and angle (@mymath{\phi}) from a fixed (but arbitrary) reference axis. In @ref{flatplane} the infinitesimal changes for each polar coordinate are plotted for a random point and a dashed circle is shown for all points with the same radius. @float Figure,flatplane @center@image{gnuastro-figures/flatplane, 10cm, , } @caption{Two dimensional Cartesian and polar coordinates on a flat plane.} @end float Assuming an object is placed at a certain position, which can be parameterized as @mymath{(x,y)}, or @mymath{(r,\phi)}, a general infinitesimal change in its position will place it in the coordinates @mymath{(x+dx,y+dy)} and @mymath{(r+dr,\phi+d\phi)}. The distance (on the flat 2D surface) that is covered by this infinitesimal change in the static universe (@mymath{ds_s}, the subscript signifies the static nature of this universe) can be written as: @dispmath{ds_s=dx^2+dy^2=dr^2+r^2d\phi^2} The main question is this: how can the 2D creature incorporate the (possible) curvature in its universe when it's calculating distances? The universe that it lives in might equally be a curved surface like @ref{sphereandplane}. The answer to this question but for a 3D being (us) is the whole purpose to this discussion. Here, we want to give the 2D creature (and later, ourselves) the tools to measure distances if the space (that hosts the objects) is curved. @ref{sphereandplane} assumes a spherical shell with radius @mymath{R} as the curved 2D plane for simplicity. The 2D plane is tangent to the spherical shell and only touches it at @mymath{A}. This idea will be generalized later. The first step in measuring the distance in a curved space is to imagine a third dimension along the @mymath{z} axis as shown in @ref{sphereandplane}. For simplicity, the @mymath{z} axis is assumed to pass through the center of the spherical shell. Our imaginary 2D creature cannot visualize the third dimension or a curved 2D surface within it, so the remainder of this discussion is purely abstract for it (similar to us having difficulty in visualizing a 3D curved space in 4D). But since we are 3D creatures, we have the advantage of visualizing the following steps. Fortunately the 2D creature is already familiar with our mathematical constructs, so it can follow our reasoning. With the third axis added, a generic infinitesimal change over @emph{the full} 3D space corresponds to the distance: @dispmath{ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2d\phi^2+dz^2.} @float Figure,sphereandplane @center@image{gnuastro-figures/sphereandplane, 10cm, , } @caption{2D spherical shell (centered on @mymath{O}) and flat plane (light gray) tangent to it at point @mymath{A}.} @end float It is very important to recognize that this change of distance is for @emph{any} point in the 3D space, not just those changes that occur on the 2D spherical shell of @ref{sphereandplane}. Recall that our 2D friend can only do measurements on the 2D surfaces, not the full 3D space. So we have to constrain this general change to any change on the 2D spherical shell. To do that, let's look at the arbitrary point @mymath{P} on the 2D spherical shell. Its image (@mymath{P'}) on the flat plain is also displayed. From the dark gray triangle, we see that @dispmath{\sin\theta={r\over R},\quad\cos\theta={R-z\over R}.}These relations allow the 2D creature to find the value of @mymath{z} (an abstract dimension for it) as a function of r (distance on a flat 2D plane, which it can visualize) and thus eliminate @mymath{z}. From @mymath{\sin^2\theta+\cos^2\theta=1}, we get @mymath{z^2-2Rz+r^2=0} and solving for @mymath{z}, we find: @dispmath{z=R\left(1\pm\sqrt{1-{r^2\over R^2}}\right).} The @mymath{\pm} can be understood from @ref{sphereandplane}: For each @mymath{r}, there are two points on the sphere, one in the upper hemisphere and one in the lower hemisphere. An infinitesimal change in @mymath{r}, will create the following infinitesimal change in @mymath{z}: @dispmath{dz={\mp r\over R}\left(1\over \sqrt{1-{r^2/R^2}}\right)dr.}Using the positive signed equation instead of @mymath{dz} in the @mymath{ds_s^2} equation above, we get: @dispmath{ds_s^2={dr^2\over 1-r^2/R^2}+r^2d\phi^2.} The derivation above was done for a spherical shell of radius @mymath{R} as a curved 2D surface. To generalize it to any surface, we can define @mymath{K=1/R^2} as the curvature parameter. Then the general infinitesimal change in a static universe can be written as: @dispmath{ds_s^2={dr^2\over 1-Kr^2}+r^2d\phi^2.} Therefore, when @mymath{K>0} (and curvature is the same everywhere), we have a finite universe, where @mymath{r} cannot become larger than @mymath{R} as in @ref{sphereandplane}. When @mymath{K=0}, we have a flat plane (@ref{flatplane}) and a negative @mymath{K} will correspond to an imaginary @mymath{R}. The latter two cases may be infinite in area (which is not a simple concept, but mathematically can be modeled with @mymath{r} extending infinitely), or finite-area (like a cylinder is flat everywhere with @mymath{ds_s^2={dx^2 + dy^2}}, but finite in one direction in size). @cindex Proper distance A very important issue that can be discussed now (while we are still in 2D and can actually visualize things) is that @mymath{\overrightarrow{r}} is tangent to the curved space at the observer's position. In other words, it is on the gray flat surface of @ref{sphereandplane}, even when the universe if curved: @mymath{\overrightarrow{r}=P'-A}. Therefore for the point @mymath{P} on a curved space, the raw coordinate @mymath{r} is the distance to @mymath{P'}, not @mymath{P}. The distance to the point @mymath{P} (at a specific coordinate @mymath{r} on the flat plane) over the curved surface (thick line in @ref{sphereandplane}) is called the @emph{proper distance} and is displayed with @mymath{l}. For the specific example of @ref{sphereandplane}, the proper distance can be calculated with: @mymath{l=R\theta} (@mymath{\theta} is in radians). using the @mymath{\sin\theta} relation found above, we can find @mymath{l} as a function of @mymath{r}: @dispmath{\theta=\sin^{-1}\left({r\over R}\right)\quad\rightarrow\quad l(r)=R\sin^{-1}\left({r\over R}\right)} @mymath{R} is just an arbitrary constant and can be directly found from @mymath{K}, so for cleaner equations, it is common practice to set @mymath{R=1}, which gives: @mymath{l(r)=\sin^{-1}r}. Also note that when @mymath{R=1}, then @mymath{l=\theta}. Generally, depending on the the curvature, in a @emph{static} universe the proper distance can be written as a function of the coordinate @mymath{r} as (from now on we are assuming @mymath{R=1}): @dispmath{l(r)=\sin^{-1}(r)\quad(K>0),\quad\quad l(r)=r\quad(K=0),\quad\quad l(r)=\sinh^{-1}(r)\quad(K<0).}With @mymath{l}, the infinitesimal change of distance can be written in a more simpler and abstract form of @dispmath{ds_s^2=dl^2+r^2d\phi^2.} @cindex Comoving distance Until now, we had assumed a static universe (not changing with time). But our observations so far appear to indicate that the universe is expanding (it isn't static). Since there is no reason to expect the observed expansion is unique to our particular position of the universe, we expect the universe to be expanding at all points with the same rate at the same time. Therefore, to add a time dependence to our distance measurements, we can include a multiplicative scaling factor, which is a function of time: @mymath{a(t)}. The functional form of @mymath{a(t)} comes from the cosmology, the physics we assume for it: general relativity, and the choice of whether the universe is uniform (`homogeneous') in density and curvature or inhomogeneous. In this section, the functional form of @mymath{a(t)} is irrelevant, so we can avoid these issues. With this scaling factor, the proper distance will also depend on time. As the universe expands, the distance between two given points will shift to larger values. We thus define a distance measure, or coordinate, that is independent of time and thus doesn't `move'. We call it the @emph{comoving distance} and display with @mymath{\chi} such that: @mymath{l(r,t)=\chi(r)a(t)}. We have therefore, shifted the @mymath{r} dependence of the proper distance we derived above for a static universe to the comoving distance: @dispmath{\chi(r)=\sin^{-1}(r)\quad(K>0),\quad\quad \chi(r)=r\quad(K=0),\quad\quad \chi(r)=\sinh^{-1}(r)\quad(K<0).} Therefore, @mymath{\chi(r)} is the proper distance to an object at a specific reference time: @mymath{t=t_r} (the @mymath{r} subscript signifies ``reference'') when @mymath{a(t_r)=1}. At any arbitrary moment (@mymath{t\neq{t_r}}) before or after @mymath{t_r}, the proper distance to the object can be scaled with @mymath{a(t)}. Measuring the change of distance in a time-dependent (expanding) universe only makes sense if we can add up space and time@footnote{In other words, making our space-time consistent with Minkowski space-time geometry. In this geometry, different observers at a given point (event) in space-time split up space-time into `space' and `time' in different ways, just like people at the same spatial position can make different choices of splitting up a map into `left--right' and `up--down'. This model is well supported by twentieth and twenty-first century observations.}. But we can only add bits of space and time together if we measure them in the same units: with a conversion constant (similar to how 1000 is used to convert a kilometer into meters). Experimentally, we find strong support for the hypothesis that this conversion constant is the speed of light (or gravitational waves@footnote{The speed of gravitational waves was recently found to be very similar to that of light in vacuum, see @url{https://arxiv.org/abs/1710.05834, arXiv:1710.05834}.}) in a vacuum. This speed is postulated to be constant@footnote{In @emph{natural units}, speed is measured in units of the speed of light in vacuum.} and is almost always written as @mymath{c}. We can thus parametrize the change in distance on an expanding 2D surface as @dispmath{ds^2=c^2dt^2-a^2(t)ds_s^2 = c^2dt^2-a^2(t)(d\chi^2+r^2d\phi^2).} @node Extending distance concepts to 3D, Invoking astcosmiccal, Distance on a 2D curved space, CosmicCalculator @subsection Extending distance concepts to 3D The concepts of @ref{Distance on a 2D curved space} are here extended to a 3D space that @emph{might} be curved. We can start with the generic infinitesimal distance in a static 3D universe, but this time in spherical coordinates instead of polar coordinates. @mymath{\theta} is shown in @ref{sphereandplane}, but here we are 3D beings, positioned on @mymath{O} (the center of the sphere) and the point @mymath{O} is tangent to a 4D-sphere. In our 3D space, a generic infinitesimal displacement will correspond to the following distance in spherical coordinates: @dispmath{ds_s^2=dx^2+dy^2+dz^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2).} Like the 2D creature before, we now have to assume an abstract dimension which we cannot visualize easily. Let's call the fourth dimension @mymath{w}, then the general change in coordinates in the @emph{full} four dimensional space will be: @dispmath{ds_s^2=dr^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)+dw^2.} @noindent But we can only work on a 3D curved space, so following exactly the same steps and conventions as our 2D friend, we arrive at: @dispmath{ds_s^2={dr^2\over 1-Kr^2}+r^2(d\theta^2+\sin^2{\theta}d\phi^2).} @noindent In a non-static universe (with a scale factor a(t)), the distance can be written as: @dispmath{ds^2=c^2dt^2-a^2(t)[d\chi^2+r^2(d\theta^2+\sin^2{\theta}d\phi^2)].} @c@dispmath{H(z){\equiv}\left(\dot{a}\over a\right)(z)=H_0E(z) } @c@dispmath{E(z)=[ \Omega_{\Lambda,0} + \Omega_{C,0}(1+z)^2 + @c\Omega_{m,0}(1+z)^3 + \Omega_{r,0}(1+z)^4 ]^{1/2}} @c Let's take @mymath{r} to be the radial coordinate of the emitting @c source, which emitted its light at redshift $z$. Then the comoving @c distance of this object would be: @c@dispmath{ \chi(r)={c\over H_0a_0}\int_0^z{dz'\over E(z')} } @c@noindent @c So the proper distance at the current time to that object is: @c @mymath{a_0\chi(r)}, therefore the angular diameter distance @c (@mymath{d_A}) and luminosity distance (@mymath{d_L}) can be written @c as: @c@dispmath{ d_A={a_0\chi(r)\over 1+z}, \quad d_L=a_0\chi(r)(1+z) } @node Invoking astcosmiccal, , Extending distance concepts to 3D, CosmicCalculator @subsection Invoking CosmicCalculator CosmicCalculator will calculate cosmological variables based on the input parameters. The executable name is @file{astcosmiccal} with the following general template @example $ astcosmiccal [OPTION...] ... @end example @noindent One line examples: @example ## Print basic cosmological properties at redshift 2.5: $ astcosmiccal -z2.5 ## Only print Comoving volume over 4pi stradian to z (Mpc^3): $ astcosmiccal --redshift=0.8 --volume ## Print luminosity distance, angular diameter distance and age ## of universe in one row at redshift 0.4 $ astcosmiccal -z0.4 -LAg ## Assume Lambda and matter density of 0.7 and 0.3 and print ## basic cosmological parameters for redshift 2.1: $ astcosmiccal -l0.7 -m0.3 -z2.1 @end example The input parameters (for example current matter density and etc) can be given as command-line options or in the configuration files, see @ref{Configuration files}. For a definition of the different parameters, please see the sections prior to this. If no redshift is given, CosmicCalculator will just print its input parameters and abort. For a full list of the input options, please see @ref{CosmicCalculator input options}. When only a redshift is given, CosmicCalculator will print all calculations (one per line) with some explanations before each. This can be good when you want a general feeling of the conditions at a specific redshift. Alternatively, if any specific calculations are requested, only the requested values will be calculated and printed with one character space between them. In this case, no description will be printed. See @ref{CosmicCalculator specific calculations} for the full list of these options along with some explanations how when/how they can be useful. @menu * CosmicCalculator input options:: Options to specify input conditions. * CosmicCalculator specific calculations:: Requesting specific outputs. @end menu @node CosmicCalculator input options, CosmicCalculator specific calculations, Invoking astcosmiccal, Invoking astcosmiccal @subsubsection CosmicCalculator input options The inputs to CosmicCalculator can be specified with the following options: @table @option @item -z FLT @itemx --redshift=FLT The redshift of interest. @item -H FLT @itemx --H0=FLT Current expansion rate (in km sec@mymath{^{-1}} Mpc@mymath{^{-1}}). @item -l FLT @itemx --olambda=FLT Cosmological constant density divided by the critical density in the current Universe (@mymath{\Omega_{\Lambda,0}}). @item -m FLT @itemx --omatter=FLT Matter (including massive neutrinos) density divided by the critical density in the current Universe (@mymath{\Omega_{m,0}}). @item -r FLT @itemx --oradiation=FLT Radiation density divided by the critical density in the current Universe (@mymath{\Omega_{r,0}}). @end table @node CosmicCalculator specific calculations, , CosmicCalculator input options, Invoking astcosmiccal @subsubsection CosmicCalculator specific calculations By default, when no specific calculations are requested, CosmicCalculator will print a complete set of all its calculators (one line for each calculation, see @ref{Invoking astcosmiccal}). The full list of calculations can be useful when you don't want any specific value, but just a general view. In other contexts (for example in a batch script or during a discussion), you know exactly what you want and don't want to be distracted by all the extra information. You can use any number of the options described below in any order. When any of these options are requested, CosmicCalculator's output will just be a single line with a single space between the (possibly) multiple values. In the example below, only the tangential distance along one arcsecond (in kpc), absolute magnitude conversion, and age of the universe at redshift 2 are printed (recall that you can merge short options together, see @ref{Options}). @example $ astcosmiccal -z2 -sag 8.585046 44.819248 3.289979 @end example Here is one example of using this feature in scripts: by adding the following two lines in a script to keep/use the comoving volume with varying redshifts: @example z=3.12 vol=$(astcosmiccal --redshift=$z --volume) @end example @cindex GNU Grep @noindent In a script, this operation might be necessary for a large number of objects (several of galaxies in a catalog for example). So the fact that all the other default calculations are ignored will also help you get to your result faster. If you are indeed dealing with many (for example thousands) of redshifts, using CosmicCalculator is not the best/fastest solution. Because it has to go through all the configuration files and preparations for each invocation. To get the best efficiency (least overhead), we recommend using Gnuastro's cosmology library (see @ref{Cosmology library}). CosmicCalculator also calls the library functions defined there for its calculations, so you get the same result with no overhead. Gnuastro also has libraries for easily reading tables into a C program, see @ref{Table input output}. Afterwards, you can easily build and run your C program for the particular processing with @ref{BuildProgram}. If you just want to inspect the value of a variable visually, the description (which comes with units) might be more useful. In such cases, the following command might be better. The other calculations will also be done, but they are so fast that you will not notice on modern computers (the time it takes your eye to focus on the result is usually longer than the processing: a fraction of a second). @example $ astcosmiccal --redshift=0.832 | grep volume @end example The full list of CosmicCalculator's specific calculations is present below. In case you have forgot the units, you can use the @option{--help} option which has the units along with a short description. @table @option @item -G @itemx --agenow The current age of the universe (given the input parameters) in Giga-years (Gyr). @item -C @itemx --criticaldensitynow The current critical density (given the input parameters) in grams per centimeter-cube (@mymath{g/cm^3}). @item -d @itemx --properdistance The proper distance (at current time) to object at the given redshift in Megaparsecs (Mpc). See @ref{Distance on a 2D curved space} for a description of the proper distance. @item -A @itemx --angulardimdist The angular diameter distance to object at given redshift in Megaparsecs (Mpc). @item -s @itemx --arcsectandist The tangential distance covered by 1 arcseconds at the given redshift in kiloparsecs (Kpc). This can be useful when trying to estimate the resolution or pixel scale of an instrument (usually in units of arcseconds) at a given redshift. @item -L @itemx --luminositydist The luminosity distance to object at given redshift in Megaparsecs (Mpc). @item -u @itemx --distancemodulus The distance modulus at given redshift. @item -a @itemx --absmagconv The conversion factor (addition) to absolute magnitude. Note that this is practically the distance modulus added with @mymath{-2.5\log{(1+z)}} for the the desired redshift based on the input parameters. Once the apparent magnitude and redshift of an object is known, this value may be added with the apparent magnitude to give the object's absolute magnitude. @item -g @itemx --age Age of the universe at given redshift in Giga-years (Gyr). @item -b @itemx --lookbacktime The look-back time to given redshift in Giga-years (Gyr). The look-back time at a given redshift is defined as the current age of the universe (@option{--agenow}) subtracted by the age of the universe at the given redshift. @item -c @itemx --criticaldensity The critical density at given redshift in grams per centimeter-cube (@mymath{g/cm^3}). @item -v @itemx --onlyvolume The comoving volume in Megaparsecs cube (Mpc@mymath{^3}) until the desired redshift based on the input parameters. @end table @node Library, Developing, High-level calculations, Top @chapter Library Each program in Gnuastro that was discussed in the prior chapters (or any program in general) is a collection of functions that is compiled into one executable file which can communicate directly with the outside world. The outside world in this context is the operating system. By communication, we mean that control is directly passed to a program from the operating system with a (possible) set of inputs and after it is finished, the program will pass control back to the operating system. For programs written in C and C++, the unique @code{main} function is in charge of this communication. Similar to a program, a library is also a collection of functions that is compiled into one executable file. However, unlike programs, libraries don't have a @code{main} function. Therefore they can't communicate directly with the outside world. This gives you the chance to write your own @code{main} function and call library functions from within it. After compiling your program into a binary executable, you just have to @emph{link} it to the library and you are ready to run (execute) your program. In this way, you can use Gnuastro at a much lower-level, and in combination with other libraries on your system, you can significantly boost your creativity. This chapter starts with a basic introduction to libraries and how you can use them in @ref{Review of library fundamentals}. The separate functions in the Gnuastro library are then introduced (classified by context) in @ref{Gnuastro library}. If you end up routinely using a fixed set of library functions, with a well-defined input and output, it will be much more beneficial if you define a program for the job. Therefore, in its @ref{Version controlled source}, Gnuastro comes with the @ref{The TEMPLATE program} to easily define your own programs(s). @menu * Review of library fundamentals:: Guide on libraries and linking. * BuildProgram:: Link and run source files with this library. * Gnuastro library:: Description of all library functions. * Library demo programs:: Demonstration for using libraries. @end menu @node Review of library fundamentals, BuildProgram, Library, Library @section Review of library fundamentals Gnuastro's libraries are written in the C programming language. In @ref{Why C}, we have thoroughly discussed the reasons behind this choice. C was actually created to write Unix, thus understanding the way C works can greatly help in effectively using programs and libraries in all Unix-like operating systems. Therefore, in the following subsections some important aspects of C, as it relates to libraries (and thus programs that depend on them) on Unix are reviewed. First we will discuss header files in @ref{Headers} and then go onto @ref{Linking}. This section finishes with @ref{Summary and example on libraries}. If you are already familiar with these concepts, please skip this section and go directly to @ref{Gnuastro library}. @cindex Modularity In theory, a full operating system (or any software) can be written as one function. Such a software would not need any headers or linking (that are discussed in the subsections below). However, writing that single function and maintaining it (adding new features, fixing bugs, documentation and etc) would be a programmer or scientist's worst nightmare! Furthermore, all the hard work that went into creating it cannot be reused in other software: every other programmer or scientist would have to re-invent the wheel. The ultimate purpose behind libraries (which come with headers and have to be linked) is to address this problem and increase modularity: ``the degree to which a system's components may be separated and recombined'' (from Wikipedia). The more modular the source code of a program or library, the easier maintaining it will be, and all the hard work that went into creating it can be reused for a wider range of problems. @menu * Headers:: Header files included in source. * Linking:: Linking the compiled source files into one. * Summary and example on libraries:: A summary and example on using libraries. @end menu @node Headers, Linking, Review of library fundamentals, Review of library fundamentals @subsection Headers @cindex Pre-Processor C source code is read from top to bottom in the source file, therefore program components (for example variables, data structures and functions) should all be @emph{defined} or @emph{declared} closer to the top of the source file: before they are used. @emph{Defining} something in C or C++ is jargon for providing its full details. @emph{Declaring} it, on the other-hand, is jargon for only providing the minimum information needed for the compiler to pass it temporarily and fill in the detailed definition later. For a function, the @emph{declaration} only contains the inputs and their data-types along with the output's type@footnote{Recall that in C, functions only have one output.}. The @emph{definition} adds to the declaration by including the exact details of what operations are done to the inputs to generate the output. As an example, take this simple summation function: @example double sum(double a, double b) @{ return a + b; @} @end example @noindent What you see above is the @emph{definition} of this function: it shows you (and the compiler) exactly what it does to the two @code{double} type inputs and that the output also has a @code{double} type. Note that a function's internal operations are rarely so simple and short, it can be arbitrarily long and complicated. This unreasonably short and simple function was chosen here for ease of reading. The declaration for this function is: @example double sum(double a, double b); @end example @noindent You can think of a function's declaration as a building's address in the city, and the definition as the building's complete blueprints. When the compiler confronts a call to a function during its processing, it doesn't need to know anything about how the inputs are processed to generate the output. Just as the postman doesn't need to know the inner structure of a building when delivering the mail. The declaration (address) is enough. Therefore by @emph{declaring} the functions once at the start of the source files, we don't have to worry about @emph{defining} them after they are used. Even for a simple real-world operation (not a simple summation like above!), you will soon need many functions (for example, some for reading/preparing the inputs, some for the processing, and some for preparing the output). Although it is technically possible, managing all the necessary functions in one file is not easy and is contrary to the modularity principle (see @ref{Review of library fundamentals}), for example the functions for preparing the input can be usable in your other projects with a different processing. Therefore, as we will see later (in @ref{Linking}), the functions don't necessarily need to be defined in the source file where they are used. As long as their definitions are ultimately linked to the final executable, everything will be fine. For now, it is just important to remember that the functions that are called within one source file must be declared within the source file (declarations are mandatory), but not necessarily defined there. In the spirit of modularity, it is common to define contextually similar functions in one source file. For example, in Gnuastro, functions that calculate the median, mean and other statistical functions are defined in @file{lib/statistics.c}, while functions that deal directly with FITS files are defined in @file{lib/fits.c}. Keeping the definition of similar functions in a separate file greatly helps their management and modularity, but this fact alone doesn't make things much easier for the caller's source code: recall that while definitions are optional, declarations are mandatory. So if this was all, the caller would have to manually copy and paste (@emph{include}) all the declarations from the various source files into the file they are working on now. To address this problem, programmers have adopted the header file convention: the header file of a source code contains all the declarations that a caller would need to be able to use any of its functions. For example, in Gnuastro, @file{lib/statistics.c} (file containing function definitions) comes with @file{lib/gnuastro/statistics.h} (only containing function declarations). The discussion above was mainly focused on functions, however, there are many more programming constructs such as pre-processor macros and data structures. Like functions, they also need to be known to the compiler when it confronts a call to them. So the header file also contains their definitions or declarations when they are necessary for the functions. @cindex Macro @cindex Structures @cindex Data structures @cindex Pre-processor macros Pre-processor macros (or macros for short) are replaced with their defined value by the pre-processor before compilation. Conventionally they are written only in capital letters to be easily recognized. It is just important to understand that the compiler doesn't see the macros, it sees their fixed values. So when a header specifies macros you can do your programming without worrying about the actual values. The standard C types (for example @code{int}, or @code{float}) are very low-level and basic. We can collect multiple C types into a @emph{structure} for a higher-level way to keep and pass-along data. See @ref{Generic data container} for some examples of macros and data structures. The contents in the header need to be @emph{include}d into the caller's source code with a special pre-processor command: @code{#include }. As the name suggests, the @emph{pre-processor} goes through the source code prior to the processor (or compiler). One of its jobs is to include, or merge, the contents of files that are mentioned with this directive in the source code. Therefore the compiler sees a single entity containing the contents of the main file and all the included files. This allows you to include many (sometimes thousands of) declarations into your code with only one line. Since the headers are also installed with the library into your system, you don't even need to keep a copy of them for each separate program, making things even more convenient. Try opening some of the @file{.c} files in Gnuastro's @file{lib/} directory with a text editor to check out the include directives at the start of the file (after the copyright notice). Let's take @file{lib/fits.c} as an example. You will notice that Gnuastro's header files (like @file{gnuastro/fits.h}) are indeed within this directory (the @file{fits.h} file is in the @file{gnuastro/} directory). You will notice that files like @file{stdio.h}, or @file{string.h} are not in this directory (or anywhere within Gnuastro). On most systems the basic C header files (like @file{stdio.h} and @file{string.h} mentioned above) are located in @file{/usr/include/}@footnote{The @file{include/} directory name is taken from the pre-processor's @code{#include} directive, which is also the motivation behind the `I' in the @option{-I} option to the pre-processor.}. Your compiler is configured to automatically search that directory (and possibly others), so you don't have to explicitly mention these directories. Go ahead, look into the @file{/usr/include} directory and find @file{stdio.h} for example. When the necessary header files are not in those specific libraries, the pre-processor can also search in places other than the current directory. You can specify those directories with this pre-processor option@footnote{Try running Gnuastro's @command{make} and find the directories given to the compiler with the @option{-I} option.}: @table @option @item -I DIR ``Add the directory @file{DIR} to the list of directories to be searched for header files. Directories named by '-I' are searched before the standard system include directories. If the directory @file{DIR} is a standard system include directory, the option is ignored to ensure that the default search order for system directories and the special treatment of system headers are not defeated...'' (quoted from the GNU Compiler Collection manual). Note that the space between @key{I} and the directory is optional and commonly not used. @end table If the pre-processor can't find the included files, it will abort with an error. In fact a common error when building programs that depend on a library is that the compiler doesn't not know where a library's header is (see @ref{Known issues}). So you have to manually tell the compiler where to look for the library's headers with the @option{-I} option. For a small software with one or two source files, this can be done manually (see @ref{Summary and example on libraries}). However, to enhance modularity, Gnuastro (and most other bin/libraries) contain many source files, so the compiler is invoked many times@footnote{Nearly every command you see being executed after running @command{make} is one call to the compiler.}. This makes manual addition or modification of this option practically impossible. @cindex GNU build system @cindex @command{CPPFLAGS} To solve this problem, in the GNU build system, there are conventional environment variables for the various kinds of compiler options (or flags). These environment variables are used in every call to the compiler (they can be empty). The environment variable used for the C Pre-Processor (or CPP) is @command{CPPFLAGS}. By giving @command{CPPFLAGS} a value once, you can be sure that each call to the compiler will be affected. See @ref{Known issues} for an example of how to set this variable at configure time. @cindex GNU build system As described in @ref{Installation directory}, you can select the top installation directory of a software using the GNU build system, when you @command{./configure} it. All the separate components will be put in their separate sub-directory under that, for example the programs, compiled libraries and library headers will go into @file{$prefix/bin} (replace @file{$prefix} with a directory), @file{$prefix/lib}, and @file{$prefix/include} respectively. For enhanced modularity, libraries that contain diverse collections of functions (like GSL, WCSLIB, and Gnuastro), put their header files in a sub-directory unique to themselves. For example all Gnuastro's header files are installed in @file{$prefix/include/gnuastro}. In your source code, you need to keep the library's sub-directory when including the headers from such libraries, for example @code{#include }@footnote{the top @file{$prefix/include} directory is usually known to the compiler}. Not all libraries need to follow this convention, for example CFITSIO only has one header (@file{fitsio.h}) which is directly installed in @file{$prefix/include}. @node Linking, Summary and example on libraries, Headers, Review of library fundamentals @subsection Linking @cindex GNU Libtool To enhance modularity, similar functions are defined in one source file (with a @file{.c} suffix, see @ref{Headers} for more). After running @command{make}, each human-readable, @file{.c} file is translated (or compiled) into a computer-readable ``object'' file (ending with @file{.o}). Note that object files are also created when building programs, they aren't particular to libraries. Try opening Gnuastro's @file{lib/} and @file{bin/progname/} directories after running @command{make} to see these object files@footnote{Gnuastro uses GNU Libtool for portable library creation. Libtool will also make a @file{.lo} file for each @file{.c} file when building libraries (@file{.lo} files are human-readable).}. Afterwards, the object files are @emph{linked} together to create an executable program or a library. @cindex GNU Binutils The object files contain the full definition of the functions in the respective @file{.c} file along with a list of any other function (or generally ``symbol'') that is referenced there. To get a list of those functions you can use the @command{nm} program which is part of GNU Binutils. For example from the top Gnuastro directory, run: @example $ nm bin/arithmetic/arithmetic.o @end example @noindent This will print a list of all the functions (more generally, `symbols') that were called within @file{bin/arithmetic/arithmetic.c} along with some further information (for example a @code{T} in the second column shows that this function is actually defined here, @code{U} says that it is undefined here). Try opening the @file{.c} file to check some of these functions for your self. Run @command{info nm} for more information. @cindex Static linking @cindex Linking: Static To recap, the @emph{compiler} created the separate object files mentioned above for each @file{.c} file. The @emph{linker} will then combine all the symbols of the various object files (and libraries) into one program or library. In the case of Arithmetic (a program) the contents of the object files in @file{bin/arithmetic/} are copied (and re-ordered) into one final executable file which we can run from the operating system. When the symbols (computer-readable function definitions in most cases) are copied into the output like this, we call the process @emph{static} linking. Let's have a closer look at static linking: we'll assume you have installed Gnuastro into the default @file{/usr/local/} directory (see @ref{Installation directory}). If you tried the @command{nm} command on one of Arithmetic's object files above, then with the command below you can confirm that all the functions that were defined in the object files (had a @code{T} in the second column) are also defined in the @file{astarithmetic} executable: @example $ nm /usr/local/bin/astarithmetic @end example @noindent But you will notice that there are still many undefined symbols (have a @code{U} in the second column). One class of such functions are Gnuastro's own library functions that start with `@code{gal_}': @example $ nm /usr/local/bin/astarithmetic | grep gal_ @end example @cindex GNU Libtool @cindex Shared library @cindex Library: shared @cindex Dynamic linking @cindex Linking: dynamic These undefined symbols (functions) will be linked to the executable every time you run arithmetic. Therefore they are known as dynamically @emph{linked} libraries @footnote{Do not confuse dynamically @emph{linked} libraries with dynamically @emph{loaded} libraries. The former (that is discussed here) are only loaded once at the program startup. However, the latter can be loaded anytime during the program's execution, they are also known as plugins.}. When the functions of a library need to be dynamically linked, the library is known as a shared library. As we saw above, static linking is done when the executable is being built. However, when a library is linked dynamically, its symbols are only checked with the available libraries at build time: they are not actually copied into the executable. Every time you run the program, the linker will be activated and will try to link the program to the installed library before it starts. If you want all the libraries to be statically linked to the executables, you have to tell Libtool (which Gnuastro uses for the linking) to disable shared libraries at configure time@footnote{Libtool is very common and is commonly used. Therefore, you can use this option to configure on most programs using the GNU build system if you want static linking.}: @example $ configure --disable-shared @end example @noindent Try configuring, statically building and installing Gnuastro with the command above. Then check the @code{gal_} symbols in the installed Arithmetic executable like before. You will see that they are actually copied this time (have a @code{T} in the second column). If the second column doesn't convince you, look at the executable file size with the following command: @example $ ls -lh /usr/local/bin/astarithmetic @end example @noindent It should be around 4.2 Megabytes with this static linking. If you configure and build Gnuastro again with shared libraries enabled (which is the default), you will notice that it is roughly 100 Kilobytes! This huge difference would have been very significant in the old days, but with the roughly Terabyte storage drives commonly in use today, it is negligible. Fortunately, output file size is not the only benefit of dynamic linking: since it links to the libraries at run-time (rather than build-time), you don't have to re-build a higher-level program or library when an update comes for one of the lower-level libraries it depends on. You just install the new low-level library and it will automatically be used next time in your higher-level tools. To be fair, this also creates a few complications@footnote{Both of these can be avoided by joining the mailing lists of the lower-level libraries and checking the changes in newer versions before installing them. Updates that result in such behaviors are generally heavily emphasized in the release notes.}: @itemize @item Reproducibility: Even though your high-level tool has the same version as before, with the updated library, you might not get the same results. @item Broken links: if some functions have been changed or removed in the updated library, then the linker will abort with an error at run-time. Therefore you need to re-build your higher-level program or library. @end itemize @cindex GNU C library To see a list of all the shared libraries that are needed for a program or a shared library to run, you can use the GNU C library's @command{ldd}@footnote{If your operating system is not using the GNU C library, you might need another tool.} program, for example: @example $ ldd /usr/local/bin/astarithmetic @end example Library file names start with a @file{lib} and end with suffix depending on their type as described below. In between these two is the name of the library, for example @file{libgnuastro.a} (Gnuastro's static library) and @file{libgsl.so.0.0.0} (GSL's shared library). @itemize @item A static library is known as an archive file and has a @file{.a} suffix. A static library is not an executable file. @item @cindex Shared library versioning @cindex Versioning: Shared library A shared library ends with a @file{.so.X.Y.Z} suffix and is executable. The three numbers in the prefix are the version of the shared library. Shared library versions are defined to allow multiple versions of a shared library simultaneously on a system and to help detect possible updates in the library and programs that depend on it by the linker. It is very important to mention that this version number is different from from the software version number (see @ref{Version numbering}), so do not confuse the two. See the ``Library interface versions'' chapter of GNU Libtool for more. For each shared library, we also have two symbolic links ending with @file{.so.X} and @file{.so}. They are automatically set by the installer, but you can change them (point them to another version of the library) when you have multiple versions on your system. @end itemize @cindex GNU Libtool For those libraries that use GNU Libtool (including Gnuastro and its dependencies), both static and dynamic libraries are built and installed in the @file{prefix/lib/} directory (see @ref{Installation directory}). In this way other programs can make which ever kind of link that they want. To link with a library, the linker needs to know where to find the library. You do that with two separate options to the linker (see @ref{Summary and example on libraries} for an example): @table @option @item -L DIR Will tell the linker to look into @file{DIR} for the libraries. For example @file{-L/usr/local/lib}, or @file{-L/home/yourname/.local/lib}. You can make multiple calls to this option, so the linker looks into several directories. Note that the space between @key{L} and the directory is optional and commonly not used. @item -lLIBRARY Specify the unique name of a library to be linked. As discussed above, library file names have fixed parts which must not be given to this option. So @option{-lgsl} will guide the linker to either look for @file{libgsl.a} or @file{libgsl.so} (depending on the type of linking it is suppose to do). You can link many libraries by repeated calls to this option. @strong{Very important: } The place of this option on the command line matters. This is often a source of confusion for beginners, so let's assume you have asked the linker to link with library A using this option. As soon as the linker confronts this option, it looks into the list of the undefined symbols it has found until that point and does a search in library A for any of those symbols. If any pending undefined symbol is found in library A, it is used. After the search in undefined symbols is complete, the contents of library A are completely discarded from the linker's memory. Therefore, if a later object file or library uses an unlinked symbol in library A, the linker will abort after it has finished its search in all the input libraries or object files. As an example, Gnuastro's @code{gal_array_dlog10_array} function depends on the @code{log10} function of the C Math library (specified with @option{-lm}). So the proper way to link something that uses this function is @option{-lgnuastro -lm}. If instead, you give: @option{-lm -lgnuastro} the linker will complain and abort. @end table @node Summary and example on libraries, , Linking, Review of library fundamentals @subsection Summary and example on libraries After the mostly abstract discussions of @ref{Headers} and @ref{Linking}, we'll give a small tutorial here. But before that, let's recall the general steps of how your source code is prepared, compiled and linked to the libraries it depends on so you can run it: @enumerate @item The @strong{pre-processor} includes the header (@file{.h}) files into the function definition (@file{.c}) files, expands pre-processor macros and generally prepares the human-readable source for compilation (reviewed in @ref{Headers}). @item The @strong{compiler} will translate (compile) the human-readable contents of each source (merged @file{.c} and the @file{.h} files, or generally the output of the pre-processor) into the computer-readable code of @file{.o} files. @item The @strong{linker} will link the called function definitions from various compiled files to create one unified object. When the unified product has a @code{main} function, this function is the product's only entry point, enabling the operating system or user to directly interact with it, so the product is a program. When the product doesn't have a @code{main} function, the linker's product is a library and its exported functions can be linked to other executables (it has many entry points). @end enumerate @cindex GCC @cindex GNU Compiler Collection The GNU Compiler Collection (or GCC for short) will do all three steps. So as a first example, from Gnuastro's source, go to @file{tests/lib/}. This directory contains the library tests, you can use these as some simple tutorials. For this demonstration, we will compile and run the @file{arraymanip.c}. This small program will call Gnuastro library for some simple operations on an array (open it and have a look). To compile this program, run this command inside the directory containing it. @example $ gcc arraymanip.c -lgnuastro -lm -o arraymanip @end example @noindent The two @option{-lgnuastro} and @option{-lm} options (in this order) tell GCC to first link with the Gnuastro library and then with C's math library. The @option{-o} option is used to specify the name of the output executable, without it the output file name will be @file{a.out} (on most OSs), independent of your input file name(s). If your top Gnuastro installation directory (let's call it @file{$prefix}, see @ref{Installation directory}) is not recognized by GCC, you will get pre-processor errors for unknown header files. Once you fix it, you will get linker errors for undefined functions. To fix both, you should run GCC as follows: additionally telling it which directories it can find Gnuastro's headers and compiled library (see @ref{Headers} and @ref{Linking}): @example $ gcc -I$prefix/include -L$prefix/lib arraymanip.c -lgnuastro -lm \ -o arraymanip @end example @noindent This single command has done all the pre-processor, compilation and linker operations. Therefore no intermediate files (object files in particular) were created, only a single output executable was created. You are now ready to run the program with: @example $ ./arraymanip @end example The Gnuastro functions called by this program only needed to be linked with the C math library. But if your program needs WCS coordinate transformations, needs to read a FITS file, needs special math operations (which include its linear algebra operations), or you want it to run on multiple CPU threads, you also need to add these libraries in the call to GCC: @option{-lgnuastro -lwcs -lcfitsio -lgsl -lgslcblas -pthread -lm}. In @ref{Gnuastro library}, where each function is documented, it is mentioned which libraries (if any) must also be linked when you call a function. If you feel all these linkings can be confusing, please consider Gnuastro's @ref{BuildProgram} program. @node BuildProgram, Gnuastro library, Review of library fundamentals, Library @section BuildProgram The number and order of libraries that are necessary for linking a program with Gnuastro library might be too confusing when you need to compile a small program for one particular job (with one source file). BuildProgram will use the information gathered during configuring Gnuastro and link with all the appropriate libraries on your system. This will allow you to easily compile, link and run programs that use Gnuastro's library with one simple command and not worry about which libraries to link to, or the linking order. @cindex GNU Libtool BuildProgram uses GNU Libtool to find the necessary libraries to link against (GNU Libtool is the same program that builds all of Gnuastro's libraries and programs when you run @code{make}). So in the future, if Gnuastro's prerequisite libraries change or other libraries are added, you don't have to worry, you can just run BuildProgram and internal linking will be done correctly. @cartouche @noindent @strong{BuildProgram requires GNU Libtool:} BuildProgram depends on GNU Libtool, other implementations don't have some necessary features. If GNU Libtool isn't available at Gnuastro's configure time, you will get a notice at the end of the configuration step and BuildProgram will not be built or installed. Please see @ref{Optional dependencies} for more information. @end cartouche @menu * Invoking astbuildprog:: Options and examples for using this program. @end menu @node Invoking astbuildprog, , BuildProgram, BuildProgram @subsection Invoking BuildProgram BuildProgram will compile and link a C source program with Gnuastro's library and all its dependencies, greatly facilitating the compilation and running of small programs that use Gnuastro's library. The executable name is @file{astbuildprog} with the following general template: @example $ astbuildprog [OPTION...] C_SOURCE_FILE @end example @noindent One line examples: @example ## Compile, link and run `myprogram.c': $ astbuildprog myprogram.c ## Similar to previous, but with optimization and compiler warnings: $ astbuildprog -Wall -O2 myprogram.c ## Compile and link `myprogram.c', then run it with `image.fits' ## as its argument: $ astbuildprog myprogram.c image.fits ## Also look in other directories for headers and linking: $ astbuildprog -Lother -Iother/dir myprogram.c ## Just build (compile and link) `myprogram.c', don't run it: $ astbuildprog --onlybuild myprogram.c @end example If BuildProgram is to run, it needs a C programming language source file as input. By default it will compile and link the program to build the a final executable file and run it. The built executable name can be set with the optional @option{--output} option. When no output name is set, BuildProgram will use Gnuastro's @ref{Automatic output}, and remove the suffix of the input and use that as the output name. For the full list of options that BuildProgram shares with other Gnuastro programs, see @ref{Common options}. You may also use Gnuastro's @ref{Configuration files} to specify other libraries/headers to use for special directories and not have to type them in every time. The first argument is considered to be the C source file that must be compiled and linked. Any other arguments (non-option tokens on the command-line) will be passed onto the program when BuildProgram wants to run it. Recall that by default BuildProgram will run the program after building it. This behavior can be disabled with the @code{--onlybuild} option. @cindex GNU Make When the @option{--quiet} option (see @ref{Operating mode options}) is not called, BuildPrograms will print the compilation and running commands. Once your program grows and you break it up into multiple files (which are much more easily managed with Make), you can use the linking flags of the non-quiet output in your @code{Makefile}. @table @option @item -I STR @itemx --includedir=STR @cindex GNU CPP @cindex C Pre-Processor Directory to search for files that you @code{#include} in your C program. Note that headers relating to Gnuastro and its dependencies don't need this option. This is only necessary if you want to use other headers. It may be called multiple times and order matters. This directory will be searched before those of Gnuastro's build and also the system search directories. See @ref{Headers} for a thorough introduction. From the GNU C Pre-Processor manual: ``Add the directory @code{STR} to the list of directories to be searched for header files. Directories named by @option{-I} are searched before the standard system include directories. If the directory @code{STR} is a standard system include directory, the option is ignored to ensure that the default search order for system directories and the special treatment of system headers are not defeated''. @item -L STR @itemx --linkdir=STR @cindex GNU Libtool Directory to search for compiled libraries to link the program with. Note that all the directories that Gnuastro was built with will already be used by BuildProgram (GNU Libtool). This option is only necessary if your libraries are in other directories. Multiple calls to this option are possible and order matters. This directory will be searched before those of Gnuastro's build and also the system search directories. See @ref{Linking} for a thorough introduction. @item -l STR @itemx --linklib=STR Library to link with your program. Note that all the libraries that Gnuastro was built with will already be linked by BuildProgram (GNU Libtool). This option is only necessary if you want to link with other directories. Multiple calls to this option are possible and order matters. This library will be linked before Gnuastro's library or its dependencies. See @ref{Linking} for a thorough introduction. @item -O INT/STR @itemx --optimize=INT/STR @cindex Optimization @cindex GNU Compiler Collection Compiler optimization level: 0 (for no optimization, good debugging), 1, 2, 3 (for the highest level of optimizations). From the GNU Compiler Collection (GCC) manual: ``Without any optimization option, the compiler's goal is to reduce the cost of compilation and to make debugging produce the expected results. Statements are independent: if you stop the program with a break point between statements, you can then assign a new value to any variable or change the program counter to any other statement in the function and get exactly the results you expect from the source code. Turning on optimization flags makes the compiler attempt to improve the performance and/or code size at the expense of compilation time and possibly the ability to debug the program.'' Please see your compiler's manual for the full list of acceptable values to this option. @item -g @itemx --debug @cindex Debug Emit extra information in the compiled binary for use by a debugger. When calling this option, it is best to explicitly disable optimization with @option{-O0}. To combine both options you can run @option{-gO0} (see @ref{Options} for how short options can be merged into one). @item -W STR @itemx --warning=STR Print compiler warnings on command-line during compilation. ``Warnings are diagnostic messages that report constructions that are not inherently erroneous but that are risky or suggest there may have been an error.'' (from the GCC manual). It is always recommended to compile your programs with warnings enabled. All compiler warning options that start with @option{W} are usable by this option in BuildProgram also, see your compiler's manual for the full list. Some of the most common values to this option are: @option{pedantic} (Warnings related to standard C) and @option{all} (all issues the compiler confronts). @item --tag=STR The language configuration information. Libtool can build objects and libraries in many languages. In many cases, it can identify the language automatically, but when it doesn't you can use this option to explicitly notify Libtool of the language. The acceptable values are: @code{CC} for C, @code{CXX} for C++, @code{GCJ} for Java, @code{F77} for Fortran 77, @code{FC} for Fortran, @code{GO} for Go and @code{RC} for Windows Resource. Note that the Gnuastro library is not yet fully compatible with all these languages. @item -b @itemx --onlybuild Only build the program, don't run it. By default, the built program is immediately run afterwards. @item --deletecompiled Delete the compiled binary file after running it. This option is only relevant when the compiled program is run after being built. In other words, it is only relevant when @option{--onlybuild} is not called. It can be useful when you are busy testing a program or just want a fast result and the actual binary/compiled file is not of later use. @item -a STR @itemx --la=STR Use the given @file{.la} file (Libtool control file) instead of the one that was produced from Gnuastro's configuration results. The Libtool control file keeps all the necessary information for building and linking a program with a library built by Libtool. The default @file{prefix/lib/libgnuastro.la} keeps all the information necessary to build a program using the Gnuastro library gathered during configure time (see @ref{Installation directory} for prefix). This option is useful when you prefer to use another Libtool control file. @end table @node Gnuastro library, Library demo programs, BuildProgram, Library @section Gnuastro library Gnuastro library's programming constructs (function declarations, macros, data structures, or global variables) are classified by context into multiple header files (see @ref{Headers})@footnote{Within Gnuastro's source, all installed @file{.h} files in @file{lib/gnuastro/} are accompanied by a @file{.c} file in @file{/lib/}.}. In this section, the functions in each header will be discussed under a separate sub-section, which includes the name of the header. Assuming a function declaration is in @file{headername.h}, you can include its declaration in your source code with: @example # include @end example @noindent The names of all constructs in @file{headername.h} are prefixed with @code{gal_headername_} (or @code{GAL_HEADERNAME_} for macros). The @code{gal_} prefix stands for @emph{G}NU @emph{A}stronomy @emph{L}ibrary. Gnuastro library functions are compiled into a single file which can be linked on the command-line with the @option{-lgnuastro} option, (see @ref{Linking} and @ref{Summary and example on libraries} for an introduction on linking and example). Gnuastro library is a high-level library which depends on lower level libraries for some operations (see @ref{Dependencies}). Therefore if at least one of Gnuastro's functions in your program use functions from the dependencies, you will also need to link those dependencies after linking with Gnuastro. The outside libraries that need to be linked for such functions are mentioned following the function name. See @ref{BuildProgram} for a small Gnuastro program that will take care of the libraries to link against and lets you focus on your exciting science. @cartouche @noindent @strong{Libraries are still under heavy development: } Gnuastro was initially created to be a collection of command-line programs. However, as the programs and their the shared functions grew, internal (not installed) libraries were added. Since the 0.2 release, the libraries are install-able. Hence the libraries are currently under heavy development and will significantly evolve between releases and will become more mature and stable in due time. It will stabilize with the removal of this notice. Check the @file{NEWS} file for interface changes. If you use the Info version of this manual (see @ref{Info}), you don't have to worry: the documentation will correspond to your installed version. @end cartouche @menu * Configuration information:: General information about library config. * Multithreaded programming:: Tools for easy multi-threaded operations. * Library data types:: Definitions and functions for types. * Library blank values:: Blank values and functions to deal with them. * Library data container:: General data container in Gnuastro. * Dimensions:: Dealing with coordinates and dimensions. * Linked lists:: Various types of linked lists. * FITS files:: Working with FITS data. * World Coordinate System:: Dealing with the world coordinate system. * Text files:: Functions to work on Text files. * Table input output:: Reading and writing table columns. * Arithmetic on datasets:: Arithmetic operations on a dataset. * Tessellation library:: Functions for working on tiles. * Bounding box:: Finding the bounding box. * Polygons:: Working with the vertices of a polygon. * Qsort functions:: Helper functions for Qsort. * Permutations:: Re-order (or permute) the values in a dataset. * Matching:: Matching catalogs based on position. * Statistical operations:: Functions for basic statistics. * Binary datasets:: Datasets that can only have values of 0 or 1. * Convolution functions:: Library functions to do convolution. * Interpolation:: Interpolate (over blank values possibly). * Git wrappers:: Wrappers for functions in libgit2. * Cosmology library:: Cosmological calculations. @end menu @node Configuration information, Multithreaded programming, Gnuastro library, Gnuastro library @subsection Configuration information (@file{config.h}) The @file{gnuastro/config.h} header contains information about the full Gnuastro installation on your system. Gnuastro developers should note that this is the only header that is not available within Gnuastro, it is only available to a Gnuastro library user @emph{after} installation. Within Gnuastro, @file{config.h} (which is included in every Gnuastro @file{.c} file, see @ref{Coding conventions}) has more than enough information about the overall Gnuastro installation. @deffn Macro GAL_CONFIG_VERSION This macro can be used as a string literal@footnote{@url{https://en.wikipedia.org/wiki/String_literal}} containing the version of Gnuastro that is being used. See @ref{Version numbering} for the version formats. For example: @example printf("Gnuastro version: %s\n", GAL_CONFIG_VERSION); @end example @noindent or @example char *gnuastro_version=GAL_CONFIG_VERSION; @end example @end deffn @deffn Macro GAL_CONFIG_HAVE_LIBGIT2 Libgit2 is an optional dependency of Gnuastro (see @ref{Optional dependencies}). When it is installed and detected at configure time, this macro will have a value of @code{1} (one). Otherwise, it will have a value of @code{0} (zero). Gnuastro also comes with some wrappers to make it easier to use libgit2 (see @ref{Git wrappers}). @end deffn @deffn Macro GAL_CONFIG_HAVE_WCSLIB_VERSION WCSLIB is the reference library for world coordinate system transformation (see @ref{WCSLIB} and @ref{World Coordinate System}). However, only more recent versions of WCSLIB also provide its version number. If the WCSLIB that is installed on the system provides its version (through the possibly existing @code{wcslib_version} function), this macro will have a value of one, otherwise it will have a value of zero. @end deffn @deffn Macro GAL_CONFIG_HAVE_PTHREAD_BARRIER The POSIX threads standard define barriers as an optional requirement. Therefore, some operating systems choose to not include it. As one of the @command{./configure} step checks, Gnuastro we check if your system has this POSIX thread barriers. If so, this macro will have a value of @code{1}, otherwise it will have a value of @code{0}. see @ref{Implementation of pthread_barrier} for more. @end deffn @cindex 32-bit @cindex 64-bit @cindex bit-32 @cindex bit-64 @deffn Macro GAL_CONFIG_SIZEOF_LONG @deffnx Macro GAL_CONFIG_SIZEOF_SIZE_T The size of (number of bytes in) the system's @code{long} and @code{size_t} types. Their values are commonly either 4 or 8 for 32-bit and 64-bit systems. You can also get this value with the expression `@code{sizeof size_t}' for example without having to include this header. @end deffn @node Multithreaded programming, Library data types, Configuration information, Gnuastro library @subsection Multithreaded programming (@file{threads.h}) @cindex Multithreaded programming In recent years, newer CPUs don't have significantly higher frequencies any more. However, CPUs are being manufactured with more cores, enabling more than one operation (thread) at each instant. This can be very useful to speed up many aspects of processing and in particular image processing. Most of the programs in Gnuastro utilize multi-threaded programming for the CPU intensive processing steps. This can potentially lead to a significant decrease in the running time of a program, see @ref{A note on threads}. In terms of reading the code, you don't need to know anything about multi-threaded programming. You can simply follow the case where only one thread is to be used. In these cases, threads are not used and can be completely ignored. @cindex POSIX threads library @cindex Lawrence Livermore National Laboratory When the C language was defined (the K&R's book was written), using threads was not common, so C's threading capabilities aren't introduced there. Gnuastro uses POSIX threads for multi-threaded programming, defined in the @file{pthread.h} system wide header. There are various resources for learning to use POSIX threads. An excellent @url{https://computing.llnl.gov/tutorials/pthreads/, tutorial} is provided by the Lawrence Livermore National Laboratory, with abundant figures to better understand the concepts, it is a very good start. The book `Advanced programming in the Unix environment'@footnote{Don't let the title scare you! The two chapters on Multi-threaded programming are very self-sufficient and don't need any more knowledge than K&R.}, by Richard Stevens and Stephen Rago, Addison-Wesley, 2013 (Third edition) also has two chapters explaining the POSIX thread constructs which can be very helpful. @cindex OpenMP An alternative to POSIX threads was OpenMP, but POSIX threads are low level, allowing much more control, while being easier to understand, see @ref{Why C}. All the situations where threads are used in Gnuastro currently are completely independent with no need of coordination between the threads. Such problems are known as ``embarrassingly parallel'' problems. They are some of the simplest problems to solve with threads and are also the ones that benefit most from them, see the LLNL introduction@footnote{@url{https://computing.llnl.gov/tutorials/parallel_comp/}}. One very useful POSIX thread concept is @code{pthread_barrier}. Unfortunately, it is only an optional feature in the POSIX standard, so some operating systems don't include it. Therefore in @ref{Implementation of pthread_barrier}, we introduce our own implementation. This is a rather technical section only necessary for more technical readers and you can safely ignore it. Following that, we describe the helper functions in this header that can greatly simplify writing a multi-threaded program, see @ref{Gnuastro's thread related functions} for more. @menu * Implementation of pthread_barrier:: Some systems don't have pthread_barrier * Gnuastro's thread related functions:: Functions for managing threads. @end menu @node Implementation of pthread_barrier, Gnuastro's thread related functions, Multithreaded programming, Multithreaded programming @subsubsection Implementation of @code{pthread_barrier} @cindex POSIX threads @cindex pthread_barrier One optional feature of the POSIX Threads standard is the @code{pthread_barrier} concept. It is a very useful high-level construct that allows for independent threads to ``wait'' behind a ``barrier'' for the rest after they finish. Barriers can thus greatly simplify the code in a multi-threaded program, so they are heavily used in Gnuastro. However, since its an optional feature in the POSIX standard, some operating systems don't include it. So to make Gnuastro portable, we have written our own implementation of those @code{pthread_barrier} functions. At @command{./configure} time, Gnuastro will check if @code{pthread_barrier} constructs are available on your system or not. If @code{pthread_barrier} is not available, our internal implementation will be compiled into the Gnuastro library and the definitions and declarations below will be usable in your code with @code{#include }. @deffn Type pthread_barrierattr_t Type to specify the attributes of a POSIX threads barrier. @end deffn @deffn Type pthread_barrier_t Structure defining the POSIX threads barrier. @end deffn @deftypefun int pthread_barrier_init (pthread_barrier_t @code{*b}, pthread_barrierattr_t @code{*attr}, unsigned int @code{limit}) Initialize the barrier @code{b}, with the attributes @code{attr} and total @code{limit} (a number of) threads that must wait behind it. This function must be called before spinning off threads. @end deftypefun @deftypefun int pthread_barrier_wait (pthread_barrier_t @code{*b}) This function is called within each thread, just before it is ready to return. Once a thread's function hits this, it will ``wait'' until all the other functions are also finished. @end deftypefun @deftypefun int pthread_barrier_destroy (pthread_barrier_t @code{*b}) Destroy all the information in the barrier structure. This should be called by the function that spinned-off the threads after all the threads have finished. @cartouche @noindent @strong{Destroy a barrier before re-using it:} It is very important to destroy the barrier before (possibly) reusing it. This destroy function not only destroys the internal structures, it also waits (in 1 microsecond intervals, so you will not notice!) until all the threads don't need the barrier structure any more. If you immediately start spinning off new threads with a not-destroyed barrier, then the internal structure of the remaining threads will get mixed with the new ones and you will get very strange and apparently random errors that are extremely hard to debug. @end cartouche @end deftypefun @node Gnuastro's thread related functions, , Implementation of pthread_barrier, Multithreaded programming @subsubsection Gnuastro's thread related functions @cindex POSIX Threads The POSIX Threads functions offered in the C library are very low-level and offer a great range of control over the properties of the threads. So if you are interested in customizing your tools for complicated thread applications, it is strongly encouraged to get a nice familiarity with them. Some resources were introduced in @ref{Multithreaded programming}. However, in many cases used in astronomical data analysis, you don't need communication between threads and each target operation can be done independently. Since such operations are very common, Gnuastro provides the tools below to facilitate the creation and management of jobs without any particular knowledge of POSIX Threads for such operations. The most interesting high-level functions of this section are the @code{gal_threads_number} and @code{gal_threads_spin_off} that identify the number of threads on the system and spin-off threads. You can see a demonstration of using these functions in @ref{Library demo - multi-threaded operation}. @deftp {C @code{struct}} gal_threads_params Structure keeping the parameters of each thread. When each thread is created, a pointer to this structure is passed to it. The @code{params} element can be the pointer to a structure defined by the user which contains all the necessary parameters to pass onto the worker function. The rest of the elements within this structure are set internally by @code{gal_threads_spin_off} and are relevant to the worker function. @example struct gal_threads_params @{ size_t id; /* Id of this thread. */ void *params; /* User-identified pointer. */ size_t *indexs; /* Target indexs given to this thread. */ pthread_barrier_t *b; /* Barrier for all threads. */ @}; @end example @end deftp @deftypefun size_t gal_threads_number () Return the number of threads that the operating system has available for your program. This number is usually fixed for a single machine and doesn't change. So this function is useful when you want to run your program on different machines (with different CPUs). @end deftypefun @deftypefun void gal_threads_spin_off (void @code{*(*worker)(void *)}, void @code{*caller_params}, size_t @code{numactions}, size_t @code{numthreads}) Distribute @code{numactions} jobs between @code{numthreads} threads and spin-off each thread by calling the @code{worker} function. The @code{caller_params} pointer will also be passed to @code{worker} as part of the @code{gal_threads_params} structure. For a fully working example of this function, please see @ref{Library demo - multi-threaded operation}. @end deftypefun @deftypefun void gal_threads_attr_barrier_init (pthread_attr_t @code{*attr}, pthread_barrier_t @code{*b}, size_t @code{limit}) @cindex Detached threads This is a low-level function in case you don't want to use @code{gal_threads_spin_off}. It will initialize the general thread attribute @code{attr} and the barrier @code{b} with @code{limit} threads to wait behind the barrier. For maximum efficiency, the threads initialized with this function will be detached. Therefore no communication is possible between these threads and in particular @code{pthread_join} won't work on these threads. You have to use the barrier constructs to wait for all threads to finish. @end deftypefun @deftypefun void gal_threads_dist_in_threads (size_t @code{numactions}, size_t @code{numthreads}, size_t @code{**outthrds}, size_t @code{*outthrdcols}) This is a low-level function in case you don't want to use @code{gal_threads_spin_off}. Identify the ``index''es (starting from 0) of the actions to be done on each thread in the @code{outthrds} array. @code{outthrds} is treated as a 2D array with @code{numthreads} rows and @code{outthrdcols} columns. The indexs in each row, identify the actions that should be done by one thread. Please see the explanation below to understand the purpose of this operation. Let's assume you have @mymath{A} actions (where there is only one function and the input values differ for each action) and @mymath{T} threads available to the system with @mymath{A>T} (common values for these two would be @mymath{A>1000} and @mymath{T<10}). Spinning off a thread is not a cheap job and requires a significant number of CPU cycles. Therefore, creating @mymath{A} threads is not the best way to address such a problem. The most efficient way to manage the actions is such that only @mymath{T} threads are created, and each thread works on a list of actions identified for it in series (one after the other). This way your CPU will get all the actions done with minimal overhead. The purpose of this function is to do what we explained above: each row in the @code{outthrds} array contains the indexs of actions which must be done by one thread. @code{outthrds} contains @code{outthrdcols} columns. In using @code{outthrds}, you don't have to know the number of columns. The @code{GAL_BLANK_SIZE_T} macro has a role very similar to a string's @code{\0}: every row finishes with this macro, so can easily stop parsing the indexes in the row when you confront it. Please see the example program in @file{tests/lib/multithread.c} for a demonstration. @end deftypefun @node Library data types, Library blank values, Multithreaded programming, Gnuastro library @subsection Library data types (@file{type.h}) Data in astronomy can have many types, numeric (numbers) and strings (names, identifiers). The former can also be divided into integers and floats, see @ref{Numeric data types} for a thorough discussion of the different numeric data types and which one is useful for different contexts. To deal with the very large diversity of types that are available (and used in different contexts), in Gnuastro each type is identified with global integer variable with a fixed name, this variable is then passed onto functions that can work on any type or is stored in Gnuastro's @ref{Generic data container} as one piece of meta-data. The actual values within these integer constants is irrelevant and you should never rely on them. When you need to check, explicitly use the named variable in the table below. If you want to check with more than one type, you can use C's @code{switch} statement. Since Gnuastro heavily deals with file input-output, the types it defines are fixed width types, these types are portable to all systems and are defined in the standard C header @file{stdint.h}. You don't need to include this header, it is included by any Gnuastro header that deals with the different types. However, the most commonly used types in a C (or C++) program (for example @code{int} or @code{long} are not defined by their exact width (storage), but by their minimum storage. So for example on some systems, @code{int} may be 2 bytes (16-bits, the minimum required by the standard) and on others it may be 4 bytes (32-bits, common in modern systems). With every type, a unique ``blank'' value (or place holder showing the absence of data) can be defined. Please see @ref{Library blank values} for constants that Gnuastro recognizes as a blank value for each type. See @ref{Numeric data types} for more explanation on the limits and particular aspects of each type. @deffn {Global integer} GAL_TYPE_INVALID This is just a place holder to specifically mark that no type has been set. @end deffn @deffn {Global integer} GAL_TYPE_BIT Identifier for a bit-stream. Currently no program in Gnuastro works directly on bits, but features will be added in the future. @end deffn @deffn {Global integer} GAL_TYPE_UINT8 Identifier for an unsigned, 8-bit integer type: @code{uint8_t} (from @file{stdint.h}), or an @code{unsigned char} in most modern systems. @end deffn @deffn {Global integer} GAL_TYPE_INT8 Identifier for a signed, 8-bit integer type: @code{int8_t} (from @file{stdint.h}), or an @code{signed char} in most modern systems. @end deffn @deffn {Global integer} GAL_TYPE_UINT16 Identifier for an unsigned, 16-bit integer type: @code{uint16_t} (from @file{stdint.h}), or an @code{unsigned short} in most modern systems. @end deffn @deffn {Global integer} GAL_TYPE_INT16 Identifier for a signed, 16-bit integer type: @code{int16_t} (from @file{stdint.h}), or a @code{short} in most modern systems. @end deffn @deffn {Global integer} GAL_TYPE_UINT32 Identifier for an unsigned, 32-bit integer type: @code{uint32_t} (from @file{stdint.h}), or an @code{unsigned int} in most modern systems. @end deffn @deffn {Global integer} GAL_TYPE_INT32 Identifier for a signed, 32-bit integer type: @code{int32_t} (from @file{stdint.h}), or an @code{int} in most modern systems. @end deffn @deffn {Global integer} GAL_TYPE_UINT64 Identifier for an unsigned, 64-bit integer type: @code{uint64_t} (from @file{stdint.h}), or an @code{unsigned long} in most modern 64-bit systems. @end deffn @deffn {Global integer} GAL_TYPE_INT64 Identifier for a signed, 64-bit integer type: @code{int64_t} (from @file{stdint.h}), or an @code{long} in most modern 64-bit systems. @end deffn @deffn {Global integer} GAL_TYPE_SIZE_T Identifier for a @code{size_t} type. This is just an alias to @code{uint32}, or @code{uint64} types for 32-bit, or 64-bit systems respectively. @end deffn @deffn {Global integer} GAL_TYPE_LONG Identifier for a @code{long} type. This is just an alias to @code{int32}, or @code{int64} types for 32-bit, or 64-bit systems respectively. @end deffn @deffn {Global integer} GAL_TYPE_FLOAT32 Identifier for a 32-bit single precision floating point type or @code{float} in C. @end deffn @deffn {Global integer} GAL_TYPE_FLOAT64 Identifier for a 64-bit double precision floating point type or @code{double} in C. @end deffn @deffn {Global integer} GAL_TYPE_COMPLEX32 Identifier for a complex number composed of two @code{float} types. Note that the complex type is not yet fully implemented in all Gnuastro's programs. @end deffn @deffn {Global integer} GAL_TYPE_COMPLEX64 Identifier for a complex number composed of two @code{double} types. Note that the complex type is not yet fully implemented in all Gnuastro's programs. @end deffn @deffn {Global integer} GAL_TYPE_STRING Identifier for a string of characters (@code{char *}). @end deffn @deffn {Global integer} GAL_TYPE_STRLL Identifier for a linked list of string of characters (@code{gal_list_str_t}, see @ref{List of strings}). @end deffn @noindent The functions below are defined to make working with the integer constants above easier. In the functions below, the constants above can be used for the @code{type} input argument. @deftypefun size_t gal_type_sizeof (uint8_t @code{type}) Return the number of bytes occupied by @code{type}. Internally, this function uses C's @code{sizeof} operator to measure the size of each type. @end deftypefun @deftypefun {char *} gal_type_name (uint8_t @code{type}, int @code{long_name}) Return a string that contains the name of @code{type}. This can be used in messages to the users when your function/program accepts many types. It can return both short and long formats of the type names (for example @code{f32} and @code{float32}). If @code{long_name} is non-zero, the long format will be returned, otherwise the short name will be returned. The output string is statically allocated, so it should not be freed. This function is the inverse of the @code{gal_type_from_name} function. For the full list of names/strings that this function will return, see @ref{Numeric data types}. @end deftypefun @deftypefun uint8_t gal_type_from_name (char @code{*str}) Return the Gnuastro integer constant that corresponds to the string @code{str}. This function is the inverse of the @code{gal_type_name} function and accepts both the short and long formats of each type. For the full list of names/strings that this function will return, see @ref{Numeric data types}. @end deftypefun @deftypefun void gal_type_min (uint8_t @code{type}, void @code{*in}) Put the minimum possible value of @code{type} in the space pointed to by @code{in}. Since the value can have any type, this function doesn't return anything, it assumes the space for the given type is available to @code{in} and writes the value there. Here is one example @example int32_t min; gal_type_min(GAL_TYPE_INT32, &min); @end example @noindent Note: Do not use the minimum value for a blank value of a general (initially unknown) type, please use the constants/functions provided in @ref{Library blank values} for the definition and usage of blank values. @end deftypefun @deftypefun void gal_type_max (uint8_t @code{type}, void @code{*in}) Put the maximum possible value of @code{type} in the space pointed to by @code{in}. Since the value can have any type, this function doesn't return anything, it assumes the space for the given type is available to @code{in} and writes the value there. Here is one example @example uint16_t max; gal_type_max(GAL_TYPE_INT16, &max); @end example @noindent Note: Do not use the maximum value for a blank value of a general (initially unknown) type, please use the constants/functions provided in @ref{Library blank values} for the definition and usage of blank values. @end deftypefun @deftypefun int gal_type_is_list (uint8_t @code{type}) Return 1 if the type is a linked list and zero otherwise. @end deftypefun @deftypefun int gal_type_out (int @code{first_type}, int @code{second_type}) Return the larger of the two given types which can be used for the type of the output of an operation involving the two input types. @end deftypefun @deftypefun {char *} gal_type_bit_string (void @code{*in}, size_t @code{size}) Return the bit-string in the @code{size} bytes that @code{in} points to. The string is dynamically allocated and must be freed afterwards. You can use it to inspect the bits within one region of memory. Here is one short example: @example int32_t a=2017; char *bitstr=gal_type_bit_string(&a, 4); printf("%d: %s (%X)\n", a, bitstr, a); free(bitstr); @end example @noindent which will produce: @example 2017: 11100001000001110000000000000000 (7E1) @end example As the example above shows, the bit-string is not the most efficient way to inspect bits. If you are familiar with hexadecimal notation, it is much more compact, see @url{https://en.wikipedia.org/wiki/Hexadecimal}. You can use @code{printf}'s @code{%x} or @code{%X} to print integers in hexadecimal format. @end deftypefun @deftypefun {char *} gal_type_to_string (void @code{*ptr}, uint8_t @code{type}, int @code{quote_if_str_has_space}); Read the contents of the memory that @code{ptr} points to (assuming it has type @code{type} and print it into an allocated string which is returned. If the memory is a string of characters and @code{quote_if_str_has_space} is non-zero, the output string will have double-quotes around it if it contains space characters. Also, note that in this case, @code{ptr} must be a pointer to an array of characters (or @code{char **}), as in the example below (which will put @code{"sample string"} into @code{out}): @example char *out, *string="sample string" out = gal_type_to_string(&string, GAL_TYPE_STRING, 1); @end example @end deftypefun @deftypefun int gal_type_from_string (void @code{**out}, char @code{*string}, uint8_t @code{type}) Read a string as a given data type and put a the pointer to it in @code{*out}. When @code{*out!=NULL}, then it is assumed to be already allocated and the value will be simply put the memory. If @code{*out==NULL}, then space will be allocated for the given type and the string will be read into that type. Note that when we are dealing with a string type, @code{*out} should be interpretted as @code{char **} (one element in an array of pointers to different strings). In other words, @code{out} should be @code{char ***}. This function can be used to fill in arrays of numbers from strings (in an already allocated data structure), or add nodes to a linked list (if the type is a list type). For an array, you have to pass the pointer to the @code{i}th element where you want the value to be stored, for example @code{&(array[i]}). If the string was successfully parsed to the requested type, this function will return a @code{0} (zero), otherwise it will return @code{1} (one). This output format will help you check the status of the conversion in a code like the example below: @example if( gal_type_from_string(&out, string, GAL_TYPE_FLOAT32) ) @{ fprintf(stderr, "%s couldn't be read as float32.\n", string); exit(EXIT_FAILURE); @} @end example @end deftypefun @deftypefun {void *} gal_type_string_to_number (char @code{*string}, uint8_t @code{*type}) Read @code{string} into smallest type that can host the number, the allocated space for the number will be returned and the type of the number will be put into the memory that @code{type} points to. If @code{string} couldn't be read as a number, this function will return @code{NULL}. For the ranges acceptable by each type see @ref{Numeric data types}. For integers it is clear, for floating point types, this function will count the number of significant digits and determine if the given string is single or double precision as described in that section. @end deftypefun @node Library blank values, Library data container, Library data types, Gnuastro library @subsection Library blank values (@file{blank.h}) When the position of an element in a dataset is important (for example a pixel in an image), a place-holder is necessary for the element if we don't have a value to fill it with (for example the CCD cannot read those pixels). We cannot simply shift all the other pixels to fill in the one we have no value for. In other cases, it often occurs that the field of sky that you are studying is not a clean rectangle to nicely fit into the boundaries of an image. You need a way to separate the pixels outside your scientific field from those inside it. Blank values act as these place holders in a dataset. They have no usable value but they have a position. @cindex NaN Every type needs a corresponding blank value (see @ref{Numeric data types} and @ref{Library data types}). Floating point types have a unique value identified by IEEE known as Not-a-Number (or NaN) which is a unique value that is recognized by the compiler. However, integer and string types don't have any standard value. For integers, in Gnuastro we take an extremum of the given type: for signed types (that allow negatives), the minimum possible value is used as blank and for unsigned types (that only accept positives), the maximum possible value is used. To be generic and easy to read/write we define a macro for these blank values and strongly encourage you only use these, and never make any assumption on the value of a type's blank value. @cindex NaN The IEEE NaN blank value type is defined to fail on any comparison, so if you are dealing with floating point types, you cannot use equality (a NaN will @emph{not} be equal to a NaN). If you know your dataset if floating point, you can use the @code{isnan} function in C's @file{math.h} header. For a description of numeric data types see @ref{Numeric data types}. For the constants identifying integers, please see @ref{Library data types}. @deffn {Global integer} GAL_BLANK_UINT8 Blank value for an unsigned, 8-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_INT8 Blank value for a signed, 8-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_UINT16 Blank value for an unsigned, 16-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_INT16 Blank value for a signed, 16-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_UINT32 Blank value for an unsigned, 32-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_INT32 Blank value for a signed, 32-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_UINT64 Blank value for an unsigned, 64-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_INT64 Blank value for a signed, 64-bit integer. @end deffn @deffn {Global integer} GAL_BLANK_SIZE_T Blank value for @code{size_t} type (@code{uint32_t} or @code{uint64_t} in 32-bit or 64-bit systems). @end deffn @cindex NaN @deffn {Global integer} GAL_BLANK_FLOAT32 Blank value for a single precision, 32-bit floating point type (IEEE NaN value). @end deffn @cindex NaN @deffn {Global integer} GAL_BLANK_FLOAT64 Blank value for a double precision, 64-bit floating point type (IEEE NaN value). @end deffn @deffn {Global integer} GAL_BLANK_STRING Blank value for string types (this is itself a string, it isn't the @code{NULL} pointer). @end deffn @noindent The functions below can be used to work with blank pixels. @deftypefun void gal_blank_write (void @code{*pointer}, uint8_t @code{type}) Write the blank value for the given @code{type} into the space that @code{pointer} points to. This can be used when the space is already allocated (for example one element in an array or a statically allocated variable). @end deftypefun @deftypefun {void *} gal_blank_alloc_write (uint8_t @code{type}) Allocate the space required to keep the blank for the given data type @code{type}, write the blank value into it and return the pointer to it. @end deftypefun @deftypefun void gal_blank_initialize (gal_data_t @code{*input}) Initialize all the elements in the @code{input} dataset to the blank value that corresponds to its type. If @code{input} is a tile over a larger dataset, only the region that the tile covers will be set to blank. @end deftypefun @deftypefun int gal_blank_present (gal_data_t @code{*input}, int @code{updateflag}) Return 1 if the dataset has a blank value and zero if it doesn't. Before checking the dataset, this function will look at @code{input}'s flags. If the @code{GAL_DATA_FLAG_HASBLANK} or @code{GAL_DATA_FLAG_DONT_CHECK_ZERO} bits of @code{input->flag} are set to 1, this function will not do any check and will just use the information in the flags. This can greatly speed up processing when a dataset needs to be checked multiple times. If you want to re-check a dataset which has non-zero flags, then explicitly set the appropriate flag to zero before calling this function. When there are no other flags, you can just set @code{input->flags} to zero, otherwise you can use this expression: @example input->flags &= ~(GAL_DATA_FLAG_HASBLANK | GAL_DATA_FLAG_USE_ZERO); @end example When @code{updateflags} is zero, this function has no side-effects on the dataset: it will not toggle the flags. When the dataset's flags were not used and @code{updateflags} is non-zero, this function will set the flags appropriately to avoid having to re-check the dataset in future calls. @end deftypefun @deftypefun {gal_data_t *} gal_blank_flag (gal_data_t @code{*input}) Create a dataset of the the same size as the input, but with an @code{uint8_t} type that has a value of 1 for data that are blank and 0 for those that aren't. @end deftypefun @deftypefun void gal_blank_remove (gal_data_t @code{*input}) Remove blank elements from a dataset, convert it to a 1D dataset, and adjust the size properly (the number of non-blank elements). In practice this function doesn't @code{realloc} the input array, it just shifts the blank elements to the end and adjusts the size elements of the @code{gal_data_t}, see @ref{Generic data container}. @end deftypefun @deftypefun {char *} gal_blank_as_string (uint8_t @code{type}, int @code{width}) Write the blank value for the given data type @code{type} into a string and return it. The space for the string is dynamically allocated so it must be freed after you are done with it. @end deftypefun @node Library data container, Dimensions, Library blank values, Gnuastro library @subsection Data container (@file{data.h}) Astronomical datasets have various dimensions, for example 1D spectra or table columns, 2D images, or 3D Integral field data cubes. Datasets can also have various numeric data types, depending on the operation/purpose, for example processed images are in commonly in floating point, but their mask images are integers using bit-wise flags to identify certain classes of special pixels, see @ref{Numeric data types}). Certain other information about a dataset are also commonly necessary, for example the units of the dataset, the name of the dataset and some comments. To deal with any generic dataset, Gnuastro defines the @code{gal_data_t} as input or output. @menu * Generic data container:: Definition of Gnuastro's generic container. * Dataset size and allocation:: Functions for size and allocation. * Arrays of datasets:: Functions to help with array of datasets. * Copying datasets:: Functions to copy a dataset to a new one. @end menu @node Generic data container, Dataset size and allocation, Library data container, Library data container @subsubsection Generic data container (@code{gal_data_t}) To be able to deal with any dataset (various dimensions, numeric data types, units and higher-level structures), Gnuastro defines the @code{gal_data_t} type which is the input/output container of choice for many of Gnuastro library's functions. It is defined in @file{gnuastro/data.h}. If you will be using (`@code{# include}'ing) those libraries, you don't need to include this header explicitly, it is already included by any library header that uses @code{gal_data_t}. @deftp {Type (C @code{struct})} gal_data_t The main container for datasets in Gnuastro. It can host data of any dimensions, with any numeric data type. It is actually a structure, but @code{typedef}'d as a new type to avoid having to write the @code{struct} before any declaration. The actual structure is shown below which is followed by a description of each element. @example typedef struct gal_data_t @{ void *restrict array; /* Basic array information. */ uint8_t type; size_t ndim; size_t *dsize; size_t size; char *mmapname; size_t minmapsize; int nwcs; /* WCS information. */ struct wcsprm *wcs; uint8_t flag; /* Content description. */ int status; char *name; char *unit; char *comment; int disp_fmt; /* For text printing. */ int disp_width; int disp_precision; struct gal_data_t *next; /* For higher-level datasets. */ struct gal_data_t *block; @} gal_data_t; @end example @end deftp @noindent The list below contains a description for each @code{gal_data_t} element. @cindex @code{void *} @table @code @item void *restrict array This is the pointer to the main array of the dataset containing the raw data (values). All the other elements in this data-structure are actually meta-data enabling us to use/understand the series of values in this array. It must allow data of any type (see @ref{Numeric data types}), so it is defined as a @code{void *} pointer. A @code{void *} array is not directly usable in C, so you have to cast it to proper type before using it, please see @ref{Library demo - reading a image} for a demonstration. @cindex @code{restrict} @cindex C: @code{restrict} The @code{restrict} keyword was formally introduced in C99 and is used to tell the compiler that at any moment only this pointer will modify what it points to (a pixel in an image for example)@footnote{Also see @url{https://en.wikipedia.org/wiki/Restrict}.}. This extra piece of information can greatly help in compiler optimizations and thus the running time of the program. But older compilers might not have this capability, so at @command{./configure} time, Gnuastro checks this feature and if the user's compiler doesn't support @code{restrict}, it will be removed from this definition. @cindex Data type @item uint8_t type A fixed code (integer) used to identify the type of data in @code{array} (see @ref{Numeric data types}). For the list of acceptable values to this variable, please see @ref{Library data types}. @item size_t ndim The dataset's number of dimensions. @cindex FORTRAN @cindex FITS standard @cindex Standard, FITS @item size_t *dsize The size of the dataset along each dimension. This is an array (with @code{ndim} elements), of positive integers in row-major order@footnote{Also see @url{https://en.wikipedia.org/wiki/Row-_and_column-major_order}.} (based on C). When a data file is read into memory with Gnuastro's libraries, this array is dynamically allocated based on the number of dimensions that the dataset has. It is important to remember that C's row-major ordering is the opposite of the FITS standard which is in column-major order: in the FITS standard the fastest dimension's size is specified by @code{NAXIS1}, and slower dimensions follow. The FITS standard was defined mainly based on the FORTRAN language which is the opposite of C's approach to multi-dimensional arrays (and also starts counting from 1 not 0). Hence if a FITS image has @code{NAXIS1==20} and @code{NAXIS2==50}, the @code{dsize} array must be filled with @code{dsize[0]==50} and @code{dsize[1]==20}. The fastest dimension is the one that is contiguous in memory: to increment by one along that dimension, just go to the next element in the array. As we go to slower dimensions, the number of memory cells we have to skip for an increment along that dimension becomes larger. @item size_t size The total number of elements in the dataset. This is actually a multiplication of all the values in the @code{dsize} array, so it is not an independent parameter. However, low-level operations with the dataset (irrespective of its dimensions) commonly need this number, so this element is designed to avoid calculating it every time. @item char *mmapname Name of file hosting the @code{mmap}'d contents of @code{array}. If the value of this variable is @code{NULL}, then the contents of @code{array} are actually stored in RAM, not in a file on the HDD/SSD. See the description of @code{minmapsize} below for more. If a file is used, it will be kept in the hidden @file{.gnuastro} directory with a randomly selected name to allow multiple arrays to be kept there at the same time. When @code{gal_data_free} is called the randomly named file will be deleted. @item size_t minmapsize The minimum size of an array (in bytes) to store the contents of @code{array} as a file (on the non-volatile HDD/SSD), not in RAM. This can be very useful for large datasets which can be very memory intensive and the user's RAM might not be sufficient to keep/process it. A random filename is assigned to the array which is available in the @code{mmapname} element of @code{gal_data_t} (above), see there for more. @code{minmapsize} is stored in each @code{gal_data_t}, so it can be passed on to subsequent/derived datasets. See the description of the @option{--minmapsize} option in @ref{Processing options} for more on using this value. @item nwcs The number of WCS coordinate representations (for WCSLIB). @item struct wcsprm *wcs The main WCSLIB structure keeping all the relevant information necessary for WCSLIB to do its processing and convert data-set positions into real-world positions. When it is given a @code{NULL} value, all possible WCS calculations/measurements will be ignored. @item uint8_t flag Bit-wise flags to describe general properties of the dataset. The number of bytes available in this flag is stored in the @code{GAL_DATA_FLAG_SIZE} macro. Note that you should use bit-wise operators@footnote{See @url{https://en.wikipedia.org/wiki/Bitwise_operations_in_C}.} to check these flags. The currently recognized bits are stored in these macros: @table @code @cindex Blank data @item GAL_DATA_FLAG_BLANK_CH Marking that the dataset has been checked for blank values. Therefore, the value of the bit in @code{GAL_DATA_FLAG_HASBLANK} is reliable. Without this bit, when a dataset doesn't have any blank values (and this has been checked), the @code{GAL_DATA_FLAG_HASBLANK} bit will be zero so a checker has no way to know if this zero is real or if no check has been done yet. @item GAL_DATA_FLAG_HASBLANK This bit has a value of @code{1} when the given dataset has blank values. If this bit is @code{0} and @code{GAL_DATA_FLAG_BLANK_CH} is @code{1}, then the dataset has been checked and it didn't have any blank values, so there is no more need for further checks. @item GAL_DATA_FLAG_SORT_CH Marking that the dataset is already checked for being sorted or not and thus that the possible @code{0} values in @code{GAL_DATA_FLAG_SORTED_I} and @code{GAL_DATA_FLAG_SORTED_D} are meaningful. @item GAL_DATA_FLAG_SORTED_I This bit has a value of @code{1} when the given dataset is sorted in an increasing manner. If this bit is @code{0} and @code{GAL_DATA_FLAG_SORT_CH} is @code{1}, then the dataset has been checked and wasn't sorted (increasing), so there is no more need for further checks. @item GAL_DATA_FLAG_SORTED_D This bit has a value of @code{1} when the given dataset is sorted in a decreasing manner. If this bit is @code{0} and @code{GAL_DATA_FLAG_SORT_CH} is @code{1}, then the dataset has been checked and wasn't sorted (decreasing), so there is no more need for further checks. @end table The macro @code{GAL_DATA_FLAG_MAXFLAG} contains the largest internally used bit-position. Higher-level flags can be defined with the bit-wise shift operators using this macro to define internal flags for libraries/programs that depend on Gnuastro without causing any possible conflict with the internal flags discussed above or having to check the values manually on every release. @item int status A context-specific status values for this data-structure. This integer will not be set by Gnuastro's libraries. You can use it keep some additional information about the dataset (with integer constants) depending on your applications. @item char *name The name of the dataset. If the dataset is a multi-dimensional array and read/written as a FITS image, this will be the value in the @code{EXTNAME} FITS keyword. If the dataset is a one-dimensional table column, this will be the column name. If it is set to @code{NULL} (by default), it will be ignored. @item char *unit The units of the dataset (for example @code{BUNIT} in the standard FITS keywords) that will be read from or written to files/tables along with the dataset. If it is set to @code{NULL} (by default), it will be ignored. @item char *comment Any further explanation about the dataset which will be written to any output file if present. @item disp_fmt Format to use for printing each element of the dataset to a plain text file, the acceptable values to this element are defined in @ref{Table input output}. Based on C's @code{printf} standards. @item disp_width Width of printing each element of the dataset to a plain text file, the acceptable values to this element are defined in @ref{Table input output}. Based on C's @code{printf} standards. @item disp_precision Precision of printing each element of the dataset to a plain text file, the acceptable values to this element are defined in @ref{Table input output}. Based on C's @code{printf} standards. @item gal_data_t *next Through this pointer, you can link a @code{gal_data_t} with other datasets related datasets, for example the different columns in a dataset each have one @code{gal_data_t} associate with them and they are linked to each other using this element. There are several functions described below to facilitate using @code{gal_data_t} as a linked list. See @ref{Linked lists} for more on these wonderful high-level constructs. @item gal_data_t *block Pointer to the start of the complete allocated block of memory. When this pointer is not @code{NULL}, the dataset is not treated as a contiguous patch of memory. Rather, it is seen as covering only a portion of the larger patch of memory that @code{block} points to. See @ref{Tessellation library} for a more thorough explanation and functions to help work with tiles that are created from this pointer. @end table @node Dataset size and allocation, Arrays of datasets, Generic data container, Library data container @subsubsection Dataset size and allocation Gnuastro's main data container was defined in @ref{Generic data container}. The functions listed in this section describe the most basic operations on @code{gal_data_t}: those related to the size, pointers, allocation and freeing. These functions are declared in @file{gnuastro/data.h} which is also visible from the function names (see @ref{Gnuastro library}). @deftypefun int gal_data_dsize_is_different (gal_data_t @code{*first}, gal_data_t @code{*second}) Return @code{1} (one) if the two datasets don't have the same size along all dimensions. This function will also return @code{1} when the number of dimensions of the two datasets are different. @end deftypefun @deftypefun {void *} gal_data_ptr_increment (void @code{*pointer}, size_t @code{increment}, uint8_t @code{type}) Return a pointer to an element that is @code{increment} elements ahead of @code{pointer}, assuming each element has type of @code{type} (for the type codes, see @ref{Library data types}). When working with the @code{array} elements of @code{gal_data_t}, we are actually dealing with @code{void *} pointers. However, pointer arithmetic doesn't apply to @code{void *}, because the system doesn't know how many bytes there are in each element to increment the pointer respectively. This function will use the given @code{type} to calculate where the incremented element is located in memory. @end deftypefun @deftypefun size_t gal_data_ptr_dist (void @code{*earlier}, void @code{*later}, uint8_t @code{type}) Return the number of elements between @code{earlier} and @code{later} assuming each element has a type defined by @code{type} (for the type codes, see @ref{Library data types}). @end deftypefun @deftypefun {void *} gal_data_malloc_array (uint8_t @code{type}, size_t @code{size}, const char @code{*funcname}, const char @code{*varname}) Allocate an array of type @code{type} with @code{size} elements in RAM (for the type codes, see @ref{Library data types}). This is effectively just a wrapper around C's @code{malloc} function but takes Gnuastro's integer type codes and will also abort with an error if there the allocation was not successful. @cindex C99 When space cannot be allocated, this function will abort the program with a message containing the reason for the failure. @code{funcname} (name of the function calling this function) and @code{varname} (name of variable that needs this space) will be used in this error message if they are not @code{NULL}. In most modern compilers, you can use the generic @code{__func__} variable for @code{funcname}. In this way, you don't have to manually copy and paste the function name or worry about it changing later (@code{__func__} was standardized in C99). @end deftypefun @deftypefun {void *} gal_data_calloc_array (uint8_t @code{type}, size_t @code{size}, const char @code{*funcname}, const char @code{*varname}) Similar to @code{gal_data_malloc_array}, but the space is cleared (set to 0) after allocation. @end deftypefun @deftypefun void gal_data_initialize (gal_data_t @code{*data}, void @code{*array}, uint8_t @code{type}, size_t @code{ndim}, size_t @code{*dsize}, struct wcsprm @code{*wcs}, int @code{clear}, size_t @code{minmapsize}, char @code{*name}, char @code{*unit}, char @code{*comment}) Initialize the given data structure (@code{data}) with all the given values. Note that the raw input @code{gal_data_t} must already have been allocated before calling this function. For a description of each variable see @ref{Generic data container}. It will set the values and do the necessary allocations. If they aren't @code{NULL}, all input arrays (@code{dsize}, @code{wcs}, @code{name}, @code{unit}, @code{comment}) are separately copied (allocated) by this function for usage in @code{data}, so you can safely use one value to initialize many datasets or use statically allocated variables in this function call. Once you are done with the dataset, you can clean all the allocated spaces with @code{gal_data_free_contents}. If @code{array} is not @code{NULL}, it will be directly copied into @code{data->array} and no new space will be allocated for the array of this dataset, this has many low-level advantages and can be used to work on regions of a dataset instead of the whole allocated array (see the description under @code{block} in @ref{Generic data container} for one example). If the given pointer is not the start of an allocated block of memory or it is used in multiple datasets, be sure to set it to @code{NULL} (with @code{data->array=NULL}) before cleaning up with @code{gal_data_free_contents}. @code{ndim} may be zero. In this case no allocation will occur, @code{data->array} and @code{data->dsize} will be set to @code{NULL} and @code{data->size} will be zero. However (when necessary) @code{dsize} must not have any zero values (a dimension of length zero is not defined). @end deftypefun @deftypefun {gal_data_t *} gal_data_alloc (void @code{*array}, uint8_t @code{type}, size_t @code{ndim}, size_t @code{*dsize}, struct wcsprm @code{*wcs}, int @code{clear}, size_t @code{minmapsize}, char @code{*name}, char @code{*unit}, char @code{*comment}) Dynamically allocate a @code{gal_data_t} and initialize it will all the given values. See the description of @code{gal_data_initialize} and @ref{Generic data container} for more information. This function will often be the most frequently used because it allocates the @code{gal_data_t} hosting all the values @emph{and} initializes it. Once you are done with the dataset, be sure to clean up all the allocated spaces with @code{gal_data_free}. @end deftypefun @deftypefun void gal_data_free_contents (gal_data_t @code{*data}) Free all the non-@code{NULL} pointers in @code{gal_data_t}. If @code{data} is actually a tile (@code{data->block!=NULL}, see @ref{Tessellation library}), then @code{tile->array} is not freed. For a complete description of @code{gal_data_t} and its contents, see @ref{Generic data container}. @end deftypefun @deftypefun void gal_data_free (gal_data_t @code{*data}) Free all the non-@code{NULL} pointers in @code{gal_data_t}, then free the actual data structure. @end deftypefun @node Arrays of datasets, Copying datasets, Dataset size and allocation, Library data container @subsubsection Arrays of datasets Gnuastro's generic data container (@code{gal_data_t}) is a very versatile structure that can be used in many higher-level contexts. One such higher-level construct is an array of @code{gal_data_t} structures to simplify the allocation (and later cleaning) of several @code{gal_data_t}s that are related. For example, each column in a table is usually represented by one @code{gal_data_t} (so it has its own name, numeric data type, units and etc). A table (with many columns) can be seen as an array of @code{gal_data_t}s (when the number of columns is known a-priori). The functions below are defined to create a cleared array of data structures and to free them in the end. These functions are declared in @file{gnuastro/data.h} which is also visible from the function names (see @ref{Gnuastro library}). @deftypefun {gal_data_t *} gal_data_array_calloc (size_t @code{size}) Allocate an array of @code{gal_data_t} with @code{size} elements. This function will also initialize all the values (@code{NULL} for pointers and 0 for other types). You can use @code{gal_data_initialize} to fill each element of the array afterwards. The following code snippet is one example of doing this. @example size_t i; gal_data_t *dataarr; dataarr=gal_data_array_calloc(10); for(i=0;i<10;++i) gal_data_initialize(&dataarr[i], ...); ... gal_data_array_free(dataarr, 10, 1); @end example @end deftypefun @deftypefun void gal_data_array_free (gal_data_t @code{*dataarr}, size_t @code{num}, int @code{free_array}) Free all the @code{num} elements within @code{dataarr} and the actual allocated array. If @code{free_array} is not zero, then the @code{array} element of all the datasets will also be freed, see @ref{Generic data container}. @end deftypefun @node Copying datasets, , Arrays of datasets, Library data container @subsubsection Copying datasets The functions in this section describes Gnuastro's facilities to copy a given dataset into another. The new dataset can have a different type (including a string), it can be already allocated (in which case only the values will be written into it). In all these cases, if the input dataset is a tile, only the data within the tile are copied. In many of the functions here, it is possible to copy the dataset to a new numeric data type (see @ref{Numeric data types}. In such cases, Gnuastro's library is going to use the native conversion by C. So if you are converting to a smaller type, it is up to you to make sure that the values fit into the output type. @deftypefun {gal_data_t *} gal_data_copy (gal_data_t @code{*in}) Return a new dataset that is a copy of @code{in}, all of @code{in}'s meta-data will also copied into the output, except for @code{block}. @end deftypefun @deftypefun {gal_data_t *} gal_data_copy_to_new_type (gal_data_t @code{*in}, uint8_t @code{newtype}) Return a copy of the dataset @code{in}, converted to @code{newtype}, see @ref{Library data types} for Gnuastro library's type identifiers. The returned dataset will have all meta-data except their type and @code{block} equal to the input's metadata. @end deftypefun @deftypefun {gal_data_t *} gal_data_copy_to_new_type_free (gal_data_t @code{*in}, uint8_t @code{newtype}) Return a copy of the dataset @code{in} that is converted to @code{newtype} and free the input dataset. See @ref{Library data types} for Gnuastro library's type identifiers. The returned dataset will have all meta-data, except their type, equal to the input's metadata. This function is similar to @code{gal_data_copy_to_new_type}, except that it will free the input dataset. @end deftypefun @deftypefun {void} gal_data_copy_to_allocated (gal_data_t @code{*in}, gal_data_t @code{*out}) Copy the contents of the array in @code{in} into the already allocated array in @code{out}. The types of the input and output may be different, type conversion will be done internally. When @code{in->size != out->size} this function will behave as follows: @table @code @item out->size < in->size This function won't re-allocate the necessary space, it will abort with an error, so please check before calling this function. @item out->size > in->size This function will write the values in @code{out->size} and @code{out->dsize} from the same values of @code{in}. So if you want to use a pre-allocated space/dataset multiple times with varying input sizes, be sure to reset @code{out->size} before every call to this function. @end table @end deftypefun @deftypefun {gal_data_t *} gal_data_copy_string_to_number (char @code{*string}) Read @code{string} into the smallest type that can store the value (see @ref{Numeric data types}). This function is just a wrapper for the @code{gal_type_string_to_number}, but will put the value into a single-element dataset. @end deftypefun @node Dimensions, Linked lists, Library data container, Gnuastro library @subsection Dimensions (@file{dimension.h}) An array is a contiguous region of memory. Hence, at the lowest level, every element of an array just has one single-valued position: the number of elements that lie between it and the first element in the array. This is also known as the @emph{index} of the element within the array. A dataset's number of dimensions is high-level abstraction (meta-data) that we project onto that contiguous patch of memory. When the array is interpreted as a one-dimensional dataset, this index is also the @emph{coordinate} of the element. But once we associate the patch of memory with a higher dimension, there must also be one coordinate for each dimension. The functions and macros in this section provide you with the tools to convert an index into a coordinate and vice-versa along with several other issues for example issues with the neighbors of an element in a multi-dimensional context. @deftypefun size_t gal_dimension_total_size (size_t @code{ndim}, size_t @code{*dsize}) Return the total number of elements for a dataset with @code{ndim} dimensions that has @code{dsize} elements along each dimension. @end deftypefun @deftypefun {size_t *} gal_dimension_increment (size_t @code{ndim}, size_t @code{*dsize}) Return an allocated array that has the number of elements necessary to increment an index along every dimension. For example along the fastest dimension (last element in the @code{dsize} and returned arrays), the value is @code{1} (one). @end deftypefun @deftypefun size_t gal_dimension_num_neighbors (size_t @code{ndim}) The maximum number of neighbors (any connectivity) that a data element can have in @code{ndim} dimensions. Effectively, this function just returns @mymath{3^n-1} (where @mymath{n} is the number of dimensions). @end deftypefun @deffn {Function-like macro} GAL_DIMENSION_FLT_TO_INT (@code{FLT}) Calculate the integer pixel position that the floating point @code{FLT} number belongs to. In the FITS format (and thus in Gnuastro), the center of each pixel is allocated on an integer (not it edge), so the pixel which hosts a floating point number cannot simply be found with internal type conversion. @end deffn @deftypefun void gal_dimension_add_coords (size_t @code{*c1}, size_t @code{*c2}, size_t @code{*out}, size_t @code{ndim}) For every dimension, add the coordinates in @code{c1} with @code{c2} and put the result into @code{out}. In other words, for dimension @code{i} run @code{out[i]=c1[i]+c2[i];}. Hence @code{out} may be equal to any one of @code{c1} or @code{c2}. @end deftypefun @deftypefun size_t gal_dimension_coord_to_index (size_t @code{ndim}, size_t @code{*dsize}, size_t @code{*coord}) Return the index (counting from zero) from the coordinates in @code{coord} (counting from zero) assuming the dataset has @code{ndim} elements and the size of the dataset along each dimension is in the @code{dsize} array. @end deftypefun @deftypefun void gal_dimension_index_to_coord (size_t @code{index}, size_t @code{ndim}, size_t @code{*dsize}, size_t @code{*coord}) Fill in the @code{coord} array with the coordinates that correspond to @code{index} assuming the dataset has @code{ndim} elements and the size of the dataset along each dimension is in the @code{dsize} array. Note that both @code{index} and each value in @code{coord} are assumed to start from @code{0} (zero). Also that the space which @code{coord} points to must already be allocated before calling this function. @end deftypefun @deftypefun size_t gal_dimension_dist_manhattan (size_t @code{*a}, size_t @code{*b}, size_t @code{ndim}) Return the manhattan distance (see @url{https://en.wikipedia.org/wiki/Taxicab_geometry, Wikipedia}) between the two coordinates @code{a} and @code{b} (each an array of @code{ndim} elements). @end deftypefun @deffn {Function-like macro} GAL_DIMENSION_NEIGHBOR_OP (@code{index}, @code{ndim}, @code{dsize}, @code{connectivity}, @code{dinc}, @code{operation}) Parse the neighbors of the element located at @code{index} and do the requested operation on them. This is defined as a macro to allow easy definition of any operation on the neighbors of a given element without having to use loops within your source code (the loops are implemented by this macro). For an example of using this function, please see @ref{Library demo - inspecting neighbors}. The input arguments to this function-like macro are described below: @table @code @item index Distance of this element from the first element in the array on a contiguous patch of memory (starting from 0), see the discussion above. @item ndim The number of dimensions associated with the contiguous patch of memory. @item dsize The full array size along each dimension. This must be an array and is assumed to have the same number elements as @code{ndim}. See the discussion under the same element in @ref{Generic data container}. @item connectivity Most distant neighbors to consider. Depending on the number of dimensions, different neighbors may be defined for each element. This function-like macro distinguish between these different neighbors with this argument. It has a value between @code{1} (one) and @code{ndim}. For example in a 2D dataset, 4-connected neighbors have a connectivity of @code{1} and 8-connected neighbors have a connectivity of @code{2}. Note that this is inclusive, so in this example, a connectivity of @code{2} will also include connectivity @code{1} neighbors. @item dinc An array keeping the length necessary to increment along each dimension. You can make this array with the following function. Just don't forget to free the array after you are done with it: @example size_t *dinc=gal_dimension_increment(ndim, dsize); @end example @code{dinc} depends on @code{ndim} and @code{dsize}, but it must be defined outside this function-like macro since it involves allocation to help in performance. @item operation Any C operation that you would like to do on the neighbor. This macro will provide you a @code{nind} variable that can be used as the index of the neighbor that is currently being studied. It is defined as `@code{size_t ndim;}'. Note that @code{operation} will be repeated the number of times there is a neighbor for this element. @end table This macro works fully within its own @code{@{@}} block and except for the @code{nind} variable that shows the neighbor's index, all the variables within this macro's block start with @code{gdn_}. @end deffn @node Linked lists, FITS files, Dimensions, Gnuastro library @subsection Linked lists (@file{list.h}) @cindex Array @cindex Linked list An array is a contiguous region of memory that is very efficient and easy to use for recording and later accessing any random element as fast as any other. This makes array the primary data container when you have many elements (for example an image which has millions of pixels). One major problem with an array is that the number of elements that go into it must be known in advance and adding or removing an element will require a re-set of all the other elements. For example if you want to remove the 3rd element in a 1000 element array, all 997 subsequent elements have to pulled back by one position, the reverse will happen if you need to add an element. In many contexts such situations never come up, for example you don't want to shift all the pixels in an image by one or two pixels from some random position in the image: their positions have scientific value. But in other contexts you will find your self frequently adding/removing an a-priori unknown number of elements. Linked lists (or @emph{lists} for short) are the data-container of choice in such situations. As in a chain, each @emph{node} in a list is an independent C structure, keeping its own data along with pointer(s) to its immediate neighbor(s). Below, you can see one simple linked list node structure along with an ASCII art schematic of how we can use the @code{next} pointer to add any number of elements to the list that we want. By convention, a list is terminated when @code{next} is the @code{NULL} pointer. @c The second and last lines lines are pushed line space forward, because @c the `@{' at the start of the line is only seen as `{' in the book. @example struct list_float /* --------- --------- */ @{ /* | Value | | Value | */ float value; /* | --- | | --- | */ struct list_float *next; /* | next-|--> | next-|--> NULL */ @} /* --------- --------- */ @end example The schematic shows another great advantage of linked lists: it is very easy to add or remove/pop a node anywhere in the list. If you want to modify the first node, you just have to change one pointer. If it is in the middle, you just have to change two. You initially define a variable of this type with a @code{NULL} pointer as shown below: @example struct list_float *mylist=NULL; @end example @noindent To add or remove/pop a node from the list you can use functions provided for the respective type in the sections below. @cindex last-in-first-out @cindex first-in-first-out @noindent When you add an element to the list, it is conventionally added to the ``top'' of the list: the general list pointer will point to the newly created node, which will point to the previously created node and so on. So when you ``pop'' from the top of the list, you are actually retrieving the last value you put in and changing the list pointer to the next youngest node. This is thus known as a ``last-in-first-out'' list. This is the most efficient type of linked list (easier to implement and faster to process). Alternatively, you can add each newly created node at the end of the list. If you do that, you will get a ``first-in-first-out'' list. But that will force you to go through the whole list for each new element that is created (this will slow down the processing)@footnote{A better way to get a first-in-first-out is to first keep the data as last-in-first-out until they are all read. Afterwards, reverse the list by popping each node and immediately add it to the new list. This practically reverses the last-in-first-out list to a first-in-first-out one. All the list types discussed in this chapter have a function with a @code{_reverse} suffix for this job.}. The node example above creates the simplest kind of a list. We can define each node with two pointers to both the next and previous neighbors, this is called a ``Doubly linked list''. In general, lists are very powerful and simple constructs that can be very useful. But going into more detail would be out of the scope of this short introduction in this book. @url{https://en.wikipedia.org/wiki/Linked_list, Wikipedia} has a nice and more thorough discussion of the various types of lists. To appreciate/use the beauty and elegance of these powerful constructs even further, see Chapter 2 (Information Structures, in volume 1) of Donald Knuth's ``The art of computer programming''. In this section we will review the functions and structures that are available in Gnuastro for working on lists. They differ by the type of data that each node can keep. For each linked-list node structure, we will first introduce the structure, then the functions for working on the structure. All these structures and functions are defined and declared in @file{gnuastro/list.h}. @menu * List of strings:: Simply linked list of strings. * List of int32_t:: Simply linked list of int32_ts. * List of size_t:: Simply linked list of size_ts. * List of float:: Simply linked list of floats. * List of double:: Simply linked list of doubles * List of void:: Simply linked list of void * pointers. * Ordered list of size_t:: Simply linked, ordered list of size_t. * Doubly linked ordered list of size_t:: Definition and functions. * List of gal_data_t:: Simply linked list Gnuastro's generic datatype. @end menu @node List of strings, List of int32_t, Linked lists, Linked lists @subsubsection List of strings Probably one of the most common lists you will be using are lists of strings. They are the best tools when you are reading the user's inputs, or when adding comments to the output files. Below you can see Gnuastro's string list type and several functions to help in adding, removing/popping, reversing and freeing the list. @deftp {Type (C @code{struct})} gal_list_str_t A single node in a list containing a string of characters. @example typedef struct gal_list_str_t @{ char *v; struct gal_list_str_t *next; @} gal_list_str_t; @end example @end deftp @deftypefun void gal_list_str_add (gal_list_str_t @code{**list}, char @code{*value}, int @code{allocate}) Add a new node to the list of strings (@code{list}) and update it. The new node will contain the string @code{value}. If @code{allocate} is not zero, space will be allocated specifically for the string of the new node and the contents of @code{value} will be copied into it. This can be useful when your string may be changed later in the program, but you want your list to remain. Here is one short/simple example of initializing and adding elements to a string list: @example gal_list_str_t *strlist; gal_list_str_add(&strlist, "bottom of list."); gal_list_str_add(&strlist, "second last element of list."); @end example @end deftypefun @deftypefun {char *} gal_list_str_pop (gal_list_str_t @code{**list}) Pop the top element of @code{list}, change @code{list} to point to the next node in the list, and return the string that was in the popped node. If @code{*list==NULL}, then this function will also return a @code{NULL} pointer. @end deftypefun @deftypefun size_t gal_list_str_number (gal_list_str_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_str_print (gal_list_str_t @code{*list}) Print the strings within each node of @code{*list} on the standard output in the same order that they are stored. Each string is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly, format. For example the following code snippet. @example size_t i; gal_list_str_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("String %zu: %s\n", i, tmp->v); @end example @end deftypefun @deftypefun void gal_list_str_reverse (gal_list_str_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun void gal_list_str_free (gal_list_str_t @code{*list}, int @code{freevalue}) Free every node in @code{list}. If @code{freevalue} is not zero, also free the string within the nodes. @end deftypefun @node List of int32_t, List of size_t, List of strings, Linked lists @subsubsection List of @code{int32_t} Signed integers are the best types when you are dealing with a positive or negative integers. The are generally useful in many contexts, for example when you want to keep the order of a series of states (each state stored as a given number in an @code{enum} for example). On many modern systems, @code{int32_t} is just an alias for @code{int}, so you can use them interchangeably. To make sure, check the size of @code{int} on your system: @deftp {Type (C @code{struct})} gal_list_i32_t A single node in a list containing a 32-bit signed integer (see @ref{Numeric data types}). @example typedef struct gal_list_i32_t @{ int32_t v; struct gal_list_i32_t *next; @} gal_list_i32_t; @end example @end deftp @deftypefun void gal_list_i32_add (gal_list_i32_t @code{**list}, int32_t @code{value}) Add a new node (containing @code{value}) to the top of the @code{list} of @code{int32_t}s (@code{uint32_t} is equal to @code{int} on many modern systems), and update @code{list}. Here is one short example of initializing and adding elements to a string list: @example gal_list_i32_t *i32list=NULL; gal_list_i32_add(&i32list, 52); gal_list_i32_add(&i32list, -4); @end example @end deftypefun @deftypefun {int32_t} gal_list_i32_pop (gal_list_i32_t @code{**list}) Pop the top element of @code{list} and return the value. This function will also change @code{list} to point to the next node in the list. If @code{*list==NULL}, then this function will also return @code{GAL_BLANK_INT32} (see @ref{Library blank values}). @end deftypefun @deftypefun size_t gal_list_i32_number (gal_list_i32_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_i32_print (gal_list_i32_t @code{*list}) Print the integers within each node of @code{*list} on the standard output in the same order that they are stored. Each integer is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. @example size_t i; gal_list_i32_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("String %zu: %s\n", i, tmp->v); @end example @end deftypefun @deftypefun void gal_list_i32_reverse (gal_list_i32_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun {int32_t *} gal_list_i32_to_array (gal_list_i32_t @code{*list}, int @code{reverse}, size_t @code{*num}) Dynamically allocate an array and fill it with the values in @code{list}. The function will return a pointer to the allocated array and put the number of elements in the array into the @code{num} pointer. If @code{reverse} has a non-zero value, the array will be filled in the opposite order of elements in @code{list}. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. @end deftypefun @deftypefun void gal_list_i32_free (gal_list_i32_t @code{*list}) Free every node in @code{list}. @end deftypefun @node List of size_t, List of float, List of int32_t, Linked lists @subsubsection List of @code{size_t} The @code{size_t} type is a unique type in C: as the name suggests it is defined to store sizes, or more accurately, the distances between memory locations. Hence it is always positive (an @code{unsigned} type) and it is directly related to the address-able spaces on the host system: on 32-bit and 64-bit systems it is an alias for @code{uint32_t} and @code{uint64_t}, respectively (see @ref{Numeric data types}). @code{size_t} is the default compiler type to index an array (recall that an array index in C is just a pointer increment of a given @emph{size}). Since it is unsigned, its a great type for counting (where negative is not defined), you are always sure it will never exceed the system's (virtual) memory and since its name has the word ``size'' inside it, it provides a good level of documentation@footnote{So you know that a variable of this type is not used to store some generic state for example.}. In Gnuastro, we do all counting and array indexing with this type, so this list is very handy. As discussed above, @code{size_t} maps to different types on different machines, so a portable way to print them with @code{printf} is to use C99's @code{%zu} format. @deftp {Type (C @code{struct})} gal_list_sizet_t A single node in a list containing a @code{size_t} value (which maps to @code{uint32_t} or @code{uint64_t} on 32-bit and 64-bit systems), see @ref{Numeric data types}. @example typedef struct gal_list_sizet_t @{ size_t v; struct gal_list_sizet_t *next; @} gal_list_sizet_t; @end example @end deftp @deftypefun void gal_list_sizet_add (gal_list_sizet_t @code{**list}, size_t @code{value}) Add a new node (containing @code{value}) to the top of the @code{list} of @code{size_t}s and update @code{list}. Here is one short example of initializing and adding elements to a string list: @example gal_list_sizet_t *slist=NULL; gal_list_sizet_add(&slist, 45493); gal_list_sizet_add(&slist, 930484); @end example @end deftypefun @deftypefun {sizet_t} gal_list_sizet_pop (gal_list_sizet_t @code{**list}) Pop the top element of @code{list} and return the value. This function will also change @code{list} to point to the next node in the list. If @code{*list==NULL}, then this function will also return @code{GAL_BLANK_SIZE_T} (see @ref{Library blank values}). @end deftypefun @deftypefun size_t gal_list_sizet_number (gal_list_sizet_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_sizet_print (gal_list_sizet_t @code{*list}) Print the values within each node of @code{*list} on the standard output in the same order that they are stored. Each integer is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example, the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. @example size_t i; gal_list_sizet_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("String %zu: %zu\n", i, tmp->v); @end example @end deftypefun @deftypefun void gal_list_sizet_reverse (gal_list_sizet_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun {size_t *} gal_list_sizet_to_array (gal_list_sizet_t @code{*list}, int @code{reverse}, size_t @code{*num}) Dynamically allocate an array and fill it with the values in @code{list}. The function will return a pointer to the allocated array and put the number of elements in the array into the @code{num} pointer. If @code{reverse} has a non-zero value, the array will be filled in the inverse of the order of elements in @code{list}. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. @end deftypefun @deftypefun void gal_list_sizet_free (gal_list_sizet_t @code{*list}) Free every node in @code{list}. @end deftypefun @node List of float, List of double, List of size_t, Linked lists @subsubsection List of @code{float} Single precision floating point numbers can accurately store real number until 7.2 decimals and only consume 4 bytes (32-bits) of memory, see @ref{Numeric data types}. Since astronomical data rarely reach that level of precision, single precision floating points are the type of choice to keep and read data. However, when processing the data, it is best to use double precision floating points (since errors propagate). @deftp {Type (C @code{struct})} gal_list_f32_t A single node in a list containing a 32-bit single precision @code{float} value: see @ref{Numeric data types}. @example typedef struct gal_list_f32_t @{ float v; struct gal_list_f32_t *next; @} gal_list_f32_t; @end example @end deftp @deftypefun void gal_list_f32_add (gal_list_f32_t @code{**list}, float @code{value}) Add a new node (containing @code{value}) to the top of the @code{list} of @code{float}s and update @code{list}. Here is one short example of initializing and adding elements to a string list: @example gal_list_f32_t *flist=NULL; gal_list_f32_add(&flist, 3.89); gal_list_f32_add(&flist, 1.23e-20); @end example @end deftypefun @deftypefun {float} gal_list_f32_pop (gal_list_f32_t @code{**list}) Pop the top element of @code{list} and return the value. This function will also change @code{list} to point to the next node in the list. If @code{*list==NULL}, then this function will return @code{GAL_BLANK_FLOAT32} (NaN, see @ref{Library blank values}). @end deftypefun @deftypefun size_t gal_list_f32_number (gal_list_f32_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_f32_print (gal_list_f32_t @code{*list}) Print the values within each node of @code{*list} on the standard output in the same order that they are stored. Each floating point number is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example, in the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. @example size_t i; gal_list_f32_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("Node %zu: %f\n", i, tmp->v); @end example @end deftypefun @deftypefun void gal_list_f32_reverse (gal_list_f32_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun {float *} gal_list_f32_to_array (gal_list_f32_t @code{*list}, int @code{reverse}, size_t @code{*num}) Dynamically allocate an array and fill it with the values in @code{list}. The function will return a pointer to the allocated array and put the number of elements in the array into the @code{num} pointer. If @code{reverse} has a non-zero value, the array will be filled in the inverse of the order of elements in @code{list}. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. @end deftypefun @deftypefun void gal_list_f32_free (gal_list_f32_t @code{*list}) Free every node in @code{list}. @end deftypefun @node List of double, List of void, List of float, Linked lists @subsubsection List of @code{double} Double precision floating point numbers can accurately store real number until 15.9 decimals and consume 8 bytes (64-bits) of memory, see @ref{Numeric data types}. This level of precision makes them very good for serious processing in the middle of a program's execution: in many cases, the propagation of errors will still be insignificant compared to actual observational errors in a data set. But since they consume 8 bytes and more CPU processing power, they are often not the best choice for storing and transferring of data. @deftp {Type (C @code{struct})} gal_list_f64_t A single node in a list containing a 64-bit double precision @code{double} value: see @ref{Numeric data types}. @example typedef struct gal_list_f64_t @{ double v; struct gal_list_f64_t *next; @} gal_list_f64_t; @end example @end deftp @deftypefun void gal_list_f64_add (gal_list_f64_t @code{**list}, double @code{value}) Add a new node (containing @code{value}) to the top of the @code{list} of @code{double}s and update @code{list}. Here is one short example of initializing and adding elements to a string list: @example gal_list_f64_t *dlist=NULL; gal_list_f64_add(&dlist, 3.8129395763193); gal_list_f64_add(&dlist, 1.239378923931e-20); @end example @end deftypefun @deftypefun {double} gal_list_f64_pop (gal_list_f64_t @code{**list}) Pop the top element of @code{list} and return the value. This function will also change @code{list} to point to the next node in the list. If @code{*list==NULL}, then this function will return @code{GAL_BLANK_FLOAT64} (NaN, see @ref{Library blank values}). @end deftypefun @deftypefun size_t gal_list_f64_number (gal_list_f64_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_f64_print (gal_list_f64_t @code{*list}) Print the values within each node of @code{*list} on the standard output in the same order that they are stored. Each floating point number is printed on one line. This function is mainly good for checking/debugging your program. For program outputs, its best to make your own implementation with a better, more user-friendly format. For example, in the following code snippet. You can also modify it to print all values in one line, and etc, depending on the context of your program. @example size_t i; gal_list_f64_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("Node %zu: %f\n", i, tmp->v); @end example @end deftypefun @deftypefun void gal_list_f64_reverse (gal_list_f64_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun {double *} gal_list_f64_to_array (gal_list_f64_t @code{*list}, int @code{reverse}, size_t @code{*num}) Dynamically allocate an array and fill it with the values in @code{list}. The function will return a pointer to the allocated array and put the number of elements in the array into the @code{num} pointer. If @code{reverse} has a non-zero value, the array will be filled in the inverse of the order of elements in @code{list}. This function can be useful after you have finished reading an initially unknown number of values and want to put them in an array for easy random access. @end deftypefun @deftypefun void gal_list_f64_free (gal_list_f64_t @code{*list}) Free every node in @code{list}. @end deftypefun @node List of void, Ordered list of size_t, List of double, Linked lists @subsubsection List of @code{void *} In C, @code{void *} is the most generic pointer. Usually pointers are associated with the type of content they point to. For example @code{int *} means a pointer to an integer. This ancillary information about the contents of the memory location is very useful for the compiler, catching bad errors and also documentation (it helps the reader see what the address in memory actually contains). However, @code{void *} is just a raw address (pointer), it contains no information on the contents it points to. These properties make the @code{void *} very useful when you want to treat the contents of an address in different ways. You can use the @code{void *} list defined in this section and its function on any kind of data: for example you can use it to keep a list of custom data structures that you have built for your own separate program. Each node in the list can keep anything and this gives you great versatility. But in using @code{void *}, please beware that ``with great power comes great responsibility''. @deftp {Type (C @code{struct})} gal_list_void_t A single node in a list containing a @code{void *} pointer. @example typedef struct gal_list_void_t @{ void *v; struct gal_list_void_t *next; @} gal_list_void_t; @end example @end deftp @deftypefun void gal_list_void_add (gal_list_void_t @code{**list}, void @code{*value}) Add a new node (containing @code{value}) to the top of the @code{list} of @code{void *}s and update @code{list}. Here is one short example of initializing and adding elements to a string list: @example gal_list_void_t *vlist=NULL; gal_list_f64_add(&vlist, some_pointer); gal_list_f64_add(&vlist, another_pointer); @end example @end deftypefun @deftypefun {void *} gal_list_void_pop (gal_list_void_t @code{**list}) Pop the top element of @code{list} and return the value. This function will also change @code{list} to point to the next node in the list. If @code{*list==NULL}, then this function will return @code{NULL}. @end deftypefun @deftypefun size_t gal_list_void_number (gal_list_void_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_void_reverse (gal_list_void_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun void gal_list_void_free (gal_list_void_t @code{*list}) Free every node in @code{list}. @end deftypefun @node Ordered list of size_t, Doubly linked ordered list of size_t, List of void, Linked lists @subsubsection Ordered list of @code{size_t} Positions/sizes in a dataset are conventionally in the @code{size_t} type (see @ref{List of size_t}) and it sometimes occurs that you want to parse and read the values in a specific order. For example you want to start from one pixel and add pixels to the list based on their distance to that pixel. So that ever time you pop an element from the list, you know it is the nearest that has not yet been studied. The @code{gal_list_osizet_t} type and its functions in this section are designed to facilitate such operations. @deftp {Type (C @code{struct})} gal_list_osizet_t @cindex @code{size_t} Each node in this singly-linked list contains a @code{size_t} value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. At any moment, the first popped node in this list will have the smallest @code{tosort} value, and subsequent nodes will have larger to values. @end deftp @example typedef struct gal_list_osizet_t @{ size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_list_osizet_t *next; @} gal_list_osizet_t; @end example @deftypefun void gal_list_osizet_add (gal_list_osizet_t @code{**list}, size_t @code{value}, float @code{tosort}) Allocate space for a new node in @code{list}, and store @code{value} and @code{tosort} into it. The new node will not necessarily be at the ``top'' of the list. If @code{*list!=NULL}, then the @code{tosort} values of existing nodes is inspected and the given node is placed in the list such that the top element (which is popped with @code{gal_list_osizet_pop}) has the smallest @code{tosort} value. @end deftypefun @deftypefun size_t gal_list_osizet_pop (gal_list_osizet_t @code{**list}, float @code{*sortvalue}) Pop a node from the top of @code{list}, return the node's @code{value} and put its sort value in the space that @code{sortvalue} points to. This function will also free the allocated space for the popped node and after this function, @code{list} will point to the next node (which has a larger @code{tosort} element). @end deftypefun @deftypefun void gal_list_osizet_to_sizet_free (gal_list_osizet_t @code{*in}, gal_list_sizet_t @code{**out}) Convert the ordered list of @code{size_t}s into an ordinary @code{size_t} linked list. This can be useful when all the elements have been added and you just need to pop-out elements and don't care about the sorting values any more. After the conversion is done, this function will free the input list. Note that the @code{out} list doesn't have to be empty. If it already contains some nodes, the new nodes will be added on top of them. @end deftypefun @node Doubly linked ordered list of size_t, List of gal_data_t, Ordered list of size_t, Linked lists @subsubsection Doubly linked ordered list of @code{size_t} An ordered list of indexs is required in many contexts, one example was discussed at the beginning of @ref{Ordered list of size_t}. But the list that was introduced there only has one point of entry: you can always only parse the list from smallest to largest. In this section, the doubly-linked @code{gal_list_dosizet_t} node is defined which will allow us to parse the values in ascending or descending order. @deftp {Type (C @code{struct})} gal_list_dosizet_t @cindex @code{size_t} Doubly-linked, ordered @code{size_t} list node structure. Each node in this Doubly-linked list contains a @code{size_t} value and a floating point value. The floating point value is used as a reference to add new nodes in a sorted manner. In the functions here, this linked list can be pointed to by two pointers (largest and smallest) with the following format: @example largest pointer | NULL <-- (v0,s0) <--> (v1,s1) <--> ... (vn,sn) --> NULL | smallest pointer @end example At any moment, the two pointers will point to the nodes containing the ``largest'' and ``smallest'' values and the rest of the nodes will be sorted. This is useful when an unknown number of nodes are being added continuously and during the operations it is important to have the nodes in a sorted format. @example typedef struct gal_list_dosizet_t @{ size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_list_dosizet_t *prev; struct gal_list_dosizet_t *next; @} gal_list_dosizet_t; @end example @end deftp @deftypefun void gal_list_dosizet_add (gal_list_dosizet_t @code{**largest}, gal_list_dosizet_t @code{**smallest}, size_t @code{value}, float @code{tosort}) Allocate space for a new node in @code{list}, and store @code{value} and @code{tosort} into it. If the list is empty, both @code{largest} and @code{smallest} must be @code{NULL}. @end deftypefun @deftypefun size_t gal_list_dosizet_pop_smallest (gal_list_dosizet_t @code{**largest}, gal_list_dosizet_t @code{**smallest}, float @code{tosort}) Pop the value with the smallest reference from the doubly linked list and store the reference into the space pointed to by @code{tosort}. Note that even though only the smallest pointer will be popped, when there was only one node in the list, the @code{largest} pointer also has to change, so we need both. @end deftypefun @deftypefun void gal_list_dosizet_print (gal_list_dosizet_t @code{*largest}, gal_list_dosizet_t @code{*smallest}) Print the largest and smallest values sequentially until the list is parsed. @end deftypefun @deftypefun void gal_list_dosizet_to_sizet (gal_list_dosizet_t @code{*in}, gal_list_sizet_t @code{**out}) Convert the doubly linked, ordered @code{size_t} list into a singly-linked list of @code{size_t}. @end deftypefun @deftypefun void gal_list_dosizet_free (gal_list_dosizet_t @code{*largest}) Free the doubly linked, ordered @code{sizet_t} list. @end deftypefun @node List of gal_data_t, , Doubly linked ordered list of size_t, Linked lists @subsubsection List of @code{gal_data_t} Gnuastro's generic data container has a @code{next} element which enables it to be used as a singly-linked list (see @ref{Generic data container}). The ability to connect the different data containers offers great advantages. For example each column in a table in an independent dataset: with its own name, units, numeric data type (see @ref{Numeric data types}). Another application is in Tessellating an input dataset into separate tiles or only studying particular regions, or tiles, of a larger dataset (see @ref{Tessellation} and @ref{Tessellation library}). Each independent tile over the dataset can be connected to the others as a linked list and thus any number of tiles can be represented with one variable. @deftypefun void gal_list_data_add (gal_data_t @code{**list}, gal_data_t @code{*newnode}) Add an already allocated dataset (@code{newnode}) to top of @code{list}. Note that if @code{newnode->next!=NULL} (@code{newnode} is itself a list), then @code{list} will be added to its end. In this example multiple images are linked together as a list: @example size_t minmapsize=-1; gal_data_t *tmp, *list=NULL; tmp = gal_fits_img_read("file1.fits", "1", minmapsize, 0, 0); gal_list_data_add( &list, tmp ); tmp = gal_fits_img_read("file2.fits", "1", minmapsize, 0, 0); gal_list_data_add( &list, tmp ); @end example @end deftypefun @deftypefun void gal_list_data_add_alloc (gal_data_t @code{**list}, void @code{*array}, uint8_t @code{type}, size_t @code{ndim}, size_t @code{*dsize}, struct wcsprm @code{*wcs}, int @code{clear}, size_t @code{minmapsize}, char @code{*name}, char @code{*unit}, char @code{*comment}) Allocate a new dataset (with @code{gal_data_alloc} in @ref{Dataset size and allocation}) and put it as the first element of @code{list}. Note that if this is the first node to be added to the list, @code{list} must be @code{NULL}. @end deftypefun @deftypefun {gal_data_t *} gal_list_data_pop (gal_data_t @code{**list}) Pop the top node from @code{list} and return it. @end deftypefun @deftypefun void gal_list_data_reverse (gal_data_t @code{**list}) Reverse the order of the list such that the top node in the list before calling this function becomes the bottom node after it. @end deftypefun @deftypefun size_t gal_list_data_number (gal_data_t @code{*list}) Return the number of nodes in @code{list}. @end deftypefun @deftypefun void gal_list_data_free (gal_data_t @code{*list}) Free all the datasets in @code{list} along with all the allocated spaces in each. @end deftypefun @node FITS files, World Coordinate System, Linked lists, Gnuastro library @subsection FITS files (@file{fits.h}) @cindex FITS @cindex CFITSIO The FITS format is the most common format to store data (images and tables) in astronomy. The CFITSIO library already provides a very good low-level collection of functions for manipulating FITS data. The low-level nature of CFITSIO is defined for versatility and portability. As a result, even a simple a basic operation, like reading an image or table column into memory, will require a special sequence of CFITSIO function calls which can be inconvenient and buggy to manage in separate locations. Therefore Gnuastro library provides wrappers for CFITSIO functions to make it much easier to read/write/modify FITS file data, header keywords and extensions. Hence, if you feel these functions don't exactly do what you want, we strongly recommend reading the CFITSIO manual to use its great features directly. All the functions and macros introduced in this section are declared in @file{gnuastro/fits.h}. When you include this header, you are also including CFITSIO's @file{fitsio.h} header. So you don't need to explicitly include @file{fitsio.h} anymore and can freely use any of its macros or functions in your code along with those discussed here. @menu * FITS macros errors filenames:: General macros, errors and checking names. * CFITSIO and Gnuastro types:: Conversion between FITS and Gnuastro types. * FITS HDUs:: Opening and getting information about HDUs. * FITS header keywords:: Reading and writing FITS header keywords. * FITS arrays:: Reading and writing FITS images/arrays. * FITS tables:: Reading and writing FITS tables. @end menu @node FITS macros errors filenames, CFITSIO and Gnuastro types, FITS files, FITS files @subsubsection FITS Macros, errors and filenames Some general constructs provided by Gnuastro's FITS handling functions are discussed here. In particular there are several useful functions about FITS file names. @deffn Macro GAL_FITS_MAX_NDIM The maximum number of dimensions a dataset can have in FITS format, according to the FITS standard this is 999. @end deffn @deftypefun void gal_fits_io_error (int @code{status}, char @code{*message}) If @code{status} is non-zero, this function will print the CFITSIO error message corresponding to status, print @code{message} (optional) in the next line and abort the program. If @code{message==NULL}, it will print a default string after the CFITSIO error. @end deftypefun @deftypefun int gal_fits_name_is_fits (char @code{*name}) If the @code{name} is an acceptable CFITSIO FITS filename return @code{1} (one), otherwise return @code{0} (zero). The currently acceptable FITS suffixes are @file{.fits}, @file{.fit}, @file{.fits.gz}, @file{.fits.Z}, @file{.imh}, @file{.fits.fz}. IMH is the IRAF format which is acceptable to CFITSIO. @end deftypefun @deftypefun int gal_fits_suffix_is_fits (char @code{*suffix}) Similar to @code{gal_fits_name_is_fits}, but only for the suffix. The suffix doesn't have to start with `@key{.}': this function will return @code{1} (one) for both @code{fits} and @code{.fits}. @end deftypefun @deftypefun {char *} gal_fits_name_save_as_string (char @code{*filename}, char @code{*hdu}) If the name is a FITS name, then put a @code{(hdu: ...)} after it and return the string. If it isn't a FITS file, just print the name. Note that the space is allocated. This function is useful when you want to report a random file to the user which may be FITS or not (for a FITS file, simply the filename is not enough, the HDU is also necessary). @end deftypefun @node CFITSIO and Gnuastro types, FITS HDUs, FITS macros errors filenames, FITS files @subsubsection CFITSIO and Gnuastro types Both Gnuastro and CFITSIO have special identifiers for each type that they accept. Gnuastro's type identifiers are fully described in @ref{Library data types} and are usable for all kinds of datasets (images, table columns and etc) as part of Gnuastro's @ref{Generic data container}. However, following the FITS standard, CFITSIO has different identifiers for images and tables. Following CFITSIO's own convention, we will use @code{bitpix} for image type identifiers and @code{datatype} for its internal identifiers (and mainly used in tables). The functions introduced in this section can be used to convert between CFITSIO and Gnuastro's type identifiers. One important issue to consider is that CFITSIO's types are not fixed width (for example @code{long} may be 32-bits or 64-bits on different systems). However, Gnuastro's types are defined by their width. These functions will use information on the host system to do the proper conversion, so it strongly recommended to use these functions for portability of your code and not to assume a fixed correspondence between CFITSIO and Gnuastro's types. @deftypefun uint8_t gal_fits_bitpix_to_type (int @code{bitpix}) Return the Gnuastro type identifier that corresponds to CFITSIO's @code{bitpix} on this system. @end deftypefun @deftypefun int gal_fits_type_to_bitpix (uint8_t @code{type}) Return the CFITSIO @code{bitpix} value that corresponds to Gnuastro's @code{type}. @end deftypefun @deftypefun char gal_fits_type_to_bin_tform (uint8_t @code{type}) Return the FITS standard binary table @code{TFORM} character that corresponds to Gnuastro's @code{type}. @end deftypefun @deftypefun int gal_fits_type_to_datatype (uint8_t @code{type}) Return the CFITSIO @code{datatype} that corresponds to Gnuastro's @code{type} on this machine. @end deftypefun @deftypefun uint8_t gal_fits_datatype_to_type (int @code{datatype}, int @code{is_table_column}) Return Gnuastro's type identifier that corresponds to the CFITSIO @code{datatype}. Note that when dealing with CFITSIO's @code{TLONG}, the fixed width type differs between tables and images. So if the corresponding dataset is a table column, put a non-zero value into @code{is_table_column}. @end deftypefun @node FITS HDUs, FITS header keywords, CFITSIO and Gnuastro types, FITS files @subsubsection FITS HDUs A FITS file can contain multiple HDUs/extensions. The functions in this section can be used to get basic information about the extensions or open them. Note that @code{fitsfile} is defined in CFITSIO's @code{fitsio.h} which is automatically included by Gnuastro's @file{gnuastro/fits.h}. @deftypefun {fitsfile *} gal_fits_open_to_write (char @code{*filename}) If @file{filename} exists, open it and return the @code{fitsfile} pointer that corresponds to it. If @file{filename} doesn't exist, the file will be created which contains a blank first extension and the pointer to its next extension will be returned. @end deftypefun @deftypefun size_t gal_fits_hdu_num (char @code{*filename}) Return the number of HDUs/extensions in @file{filename}. @end deftypefun @deftypefun int gal_fits_hdu_format (char @code{*filename}, char @code{*hdu}) Return the format of the HDU as one of CFITSIO's recognized macros: @code{IMAGE_HDU}, @code{ASCII_TBL}, or @code{BINARY_TBL}. @end deftypefun @deftypefun {fitsfile *} gal_fits_hdu_open (char @code{*filename}, char @code{*hdu}, int @code{iomode}) Open the HDU/extension @code{hdu} from @file{filename} and return a pointer to CFITSIO's @code{fitsfile}. @code{iomode} determines how the FITS file will be opened using CFITSIO's macros: @code{READONLY} or @code{READWRITE}. The string in @code{hdu} will be appended to @file{filename} in square brackets so CFITSIO only opens this extension. You can use any formatting for the @code{hdu} that is acceptable to CFITSIO. See the description under @option{--hdu} in @ref{Input output options} for more. @end deftypefun @deftypefun {fitsfile *} gal_fits_hdu_open_format (char @code{*filename}, char @code{*hdu}, int @code{img0_tab1}) Open (in read-only format) the @code{hdu} HDU/extension of @file{filename} as an image or table. When @code{img0_tab1} is @code{0}(zero) but the HDU is a table, this function will abort with an error. It will also abort with an error when @code{img0_tab1} is @code{1} (one), but the HDU is an image. A FITS HDU may contain both tables or images. When your program needs one of these formats, you can call this function so if the user provided the wrong HDU/file, it will abort and inform the user that the file/HDU is has the wrong format. @end deftypefun @node FITS header keywords, FITS arrays, FITS HDUs, FITS files @subsubsection FITS header keywords Each FITS extension/HDU contains a raw dataset which can either be a table or an image along with some header keywords. The keywords can be used to store meta-data about the actual dataset. The functions in this section describe Gnuastro's high-level functions for reading and writing FITS keywords. Similar to all Gnuastro's FITS-related functions, these functions are all wrappers for CFITSIO's low-level functions. The necessary meta-data (header keywords) for a particular dataset are commonly numerous, it is much more efficient to list them in one variable and call the reading/writing functions once. Hence the functions in this section use linked lists, a thorough introduction to them is given in @ref{Linked lists}. To reading FITS keywords, these functions use a list of Gnuastro's generic dataset format that is discussed in @ref{List of gal_data_t}. To write FITS keywords we define the @code{gal_fits_list_key_t} node that is defined below. @deftp {Type (C @code{struct})} gal_fits_list_key_t @cindex Linked list @cindex last-in-first-out @cindex first-in-first-out Structure for writing FITS keywords. This structure is used for one keyword and you don't need to set all elements. With the @code{next} element, you can link it to another keyword thus creating a linked list to add any number of keywords easily and at any step during your program (see @ref{Linked lists} for an introduction on lists). See the functions below for adding elements to the list. @example typedef struct gal_fits_list_key_t @{ int kfree; /* ==1, free name. */ int vfree; /* ==1, free value. */ int cfree; /* ==1, free comment. */ uint8_t type; /* Keyword value type. */ char *keyname; /* Keyword Name. */ void *value; /* Keyword value. */ char *comment; /* Keyword comment. */ char *unit; /* Keyword unit. */ struct gal_fits_list_key_t *next; /* Next keyword. */ @} gal_fits_list_key_t; @end example @end deftp @deftypefun {void *} gal_fits_key_img_blank (uint8_t @code{type}) Returns a pointer to an allocated space for the FITS @code{BLANK} header keyword when the input array has a type of @code{type}. According to the FITS standard: ``If the @code{BSCALE} and @code{BZERO} keywords do not have the default values of 1.0 and 0.0, respectively, then the value of the @code{BLANK} keyword must equal the actual value in the FITS data array that is used to represent an undefined pixel and not the corresponding physical value''. Therefore a special @code{BLANK} value is needed for datasets containing signed 8-bit integers and unsigned 16-bit, 32-bit and 64-bit integers (types that are defined with @code{BSCALE} and @code{BZERO} in the FITS standard). @end deftypefun @deftypefun void gal_fits_key_clean_str_value (char @code{*string}) Remove the single quotes and possible extra spaces around the keyword values that CFITSIO returns when reading a string keyword. CFITSIO doesn't remove the two single quotes around the string value of a keyword. Hence the strings it reads are like: @code{'value '}, or @code{'some_very_long_value'}. To use the value during your processing, it is commonly necessary to remove the single quotes (and possible extra spaces). This function will do this within the allocated space of the string. @end deftypefun @deftypefun void gal_fits_key_read_from_ptr (fitsfile @code{*fptr}, gal_data_t @code{*keysll}, int @code{readcomment}, int @code{readunit}) Read the list of keyword values from a FITS pointer. The input should be a linked list of Gnuastro's generic data container (@code{gal_data_t}). Before calling this function, you just have to set the @code{name} and desired @code{type} values of each node in the list to the keyword you want it to keep the value of. The given @code{name} value will be directly passed to CFITSIO to read the desired keyword name. This function will allocate space to keep the value. If @code{readcomment} and @code{readunit} are non-zero, this function will also try to read the possible comments and units of the keyword. Here is one example of using this function: @example /* Allocate an array of datasets. */ gal_data_t *keysll=gal_data_array_calloc(N); /* Use the array as a list.*/ for(i=0;i0) and used as the keyword name. The FITS standard sets a maximum length for the value of a keyword. This creates problems with file names (which include directories). Because file names/addresses can become very long. Therefore, when @code{filename} is longer than the maximum length of a FITS keyword value, this function will break it into several keywords (breaking up the string on directory separators). @end deftypefun @deftypefun void gal_fits_key_write_wcsstr (fitsfile @code{*fptr}, char @code{*wcsstr}, int @code{nkeyrec}) Write the WCS header string (produced with WCSLIB's @code{wcshdo} function) into the CFITSIO @code{fitsfile} pointer. @code{nkeyrec} is the number of FITS header keywords in @code{wcsstr}. This function will put a few blank keyword lines along with a comment @code{WCS information} before writing each keyword record. @end deftypefun @deftypefun void gal_fits_key_write (fitsfile @code{*fptr}, gal_fits_list_key_t @code{**keylist}) Write the list of keywords in @code{keylist} into the CFITSIO @code{fitsfile}. @end deftypefun @deftypefun void gal_fits_key_write_version (fitsfile @code{*fptr}, gal_fits_list_key_t @code{*headers}, char @code{*program_name}) Write or update (all the) keyword(s) in @code{headers} into the FITS pointer, but also the date, name of your program (@code{program_name}), along with the versions of CFITSIO, WCSLIB (when available), GSL, Gnuastro, and (the possible) commit information into the header as described in @ref{Output headers}. Since the data processing depends on the versions of the libraries you have used, it is strongly recommended to include this information in every FITS output. @code{gal_fits_img_write} and @code{gal_fits_tab_write} will automatically use this function. @end deftypefun @node FITS arrays, FITS tables, FITS header keywords, FITS files @subsubsection FITS arrays (images) Images (or multi-dimensional arrays in general) are one of the common data formats that is stored in FITS files. Only one image may be stored in each FITS HDU/extension. The functions described here can be used to get the information of, read, or write images in FITS files. @deftypefun void gal_fits_img_info (fitsfile @code{*fptr}, int @code{*type}, size_t @code{*ndim}, size_t @code{**dsize}, char @code{**name}, char @code{**unit}) Read the type (see @ref{Library data types}), number of dimensions, and size along each dimension of the CFITSIO @code{fitsfile} into the @code{type}, @code{ndim}, and @code{dsize} pointers respectively. If @code{name} and @code{unit} are not @code{NULL} (point to a @code{char *}), then if the image has a name and units, the respective string will be put in these pointers. @end deftypefun @deftypefun {gal_data_t *} gal_fits_img_read (char @code{*filename}, char @code{*hdu}, size_t @code{minmapsize}, size_t @code{hstartwcs}, size_t @code{hendwcs}) Read the contents of the @code{hdu} extension/HDU of @code{filename} into a Gnuastro generic data container (see @ref{Generic data container}) and return it. If the necessary space is larger than @code{minmapsize}, then don't keep the data in RAM, but in a file on the HDD/SSD. For more on @code{minmapsize} see the description under the same name in @ref{Generic data container}. The @code{hstartwcs} and @code{hendwcs} arguments are the starting and ending header keywords to search for WCS information, if no limit is needed, set them to zero. For more on these two options, please see the description of @code{gal_wcs_read_fitsptr} in @ref{World Coordinate System}. @end deftypefun @deftypefun {gal_data_t *} gal_fits_img_read_to_type (char @code{*inputname}, char @code{*inhdu}, uint8_t @code{type}, size_t @code{minmapsize}, ) Read the contents of the @code{hdu} extension/HDU of @code{filename} into a Gnuastro generic data container (see @ref{Generic data container}) of type @code{type} and return it. This is just a wrapper around @code{gal_fits_img_read} (to read the image/array of any type) and @code{gal_data_copy_to_new_type_free} (to convert it to @code{type} and free the initially read dataset). See the description there for more. @end deftypefun @cindex NaN @cindex Convolution kernel @cindex Kernel, convolution @deftypefun {gal_data_t *} gal_fits_img_read_kernel (char @code{*filename}, char @code{*hdu}, size_t @code{minmapsize}) Read the @code{hdu} of @code{filename} as a convolution kernel. A convolution kernel must have an odd size along all dimensions, it must not have blank (NaN in floating point types) values and must be flipped around the center to make the proper convolution (see @ref{Convolution process}). If there are blank values, this function will change the blank values to @code{0.0}. If the input image doesn't have the other two requirements, this function will abort with an error describing the condition to the user. The finally returned dataset will have a @code{float32} type. @end deftypefun @deftypefun {fitsfile *} gal_fits_img_write_to_ptr (gal_data_t @code{*input}, char @code{*filename}) Write the @code{input} dataset into a FITS file named @file{filename} and return the corresponding CFITSIO @code{fitsfile} pointer. This function won't close @code{fitsfile}, so you can still add other extensions to it after this function or make other modifications. @end deftypefun @deftypefun void gal_fits_img_write (gal_data_t @code{*data}, char @code{*filename}, gal_fits_list_key_t @code{*headers}, char @code{*program_string}) Write the @code{input} dataset into the FITS file named @file{filename}. Also add the @code{headers} keywords to the newly created HDU/extension it along with your program's name (@code{program_string}). @end deftypefun @deftypefun void gal_fits_img_write_to_type (gal_data_t @code{*data}, char @code{*filename}, gal_fits_list_key_t @code{*headers}, char @code{*program_string}, int @code{type}) Convert the @code{input} dataset into @code{type}, then write it into the FITS file named @file{filename}. Also add the @code{headers} keywords to the newly created HDU/extension along with your program's name (@code{program_string}). After the FITS file is written, this function will free the copied dataset (with type @code{type}) from memory. This is just a wrapper for the @code{gal_data_copy_to_new_type} and @code{gal_fits_img_write} functions. @end deftypefun @deftypefun void gal_fits_img_write_corr_wcs_str (gal_data_t @code{*data}, char @code{*filename}, char @code{*wcsstr}, int @code{nkeyrec}, double @code{*crpix}, gal_fits_list_key_t @code{*headers}, char @code{*program_string}) Write the @code{input} dataset into @file{filename} using the @code{wcsstr} while correcting the @code{CRPIX} values. This function is mainly useful when you want to make FITS files in parallel (from one main WCS structure, with just differing CRPIX). This can happen in the following cases for example: @itemize @item When a large number of FITS images (with WCS) need to be created in parallel, it can be much more efficient to write the header's WCS keywords once at first, write them in the FITS file, then just correct the CRPIX values. @item WCSLIB's header writing function is not thread safe. So when writing FITS images in parallel, we can't write the header keywords in each thread. @end itemize @end deftypefun @node FITS tables, , FITS arrays, FITS files @subsubsection FITS tables Tables are one of the common formats of data that is stored in FITS files. Only one table may be stored in each FITS HDU/extension, but each table column must be viewed as a different dataset (with its own name, units and numeric data type for example). The only constraint of the column datasets in a table is that they must be one-dimensional and have the same number of elements as the other columns. The functions described here can be used to get the information of, read, or write columns into FITS tables. @deftypefun void gal_fits_tab_size (fitsfile @code{*fitsptr}, size_t @code{*nrows}, size_t @code{*ncols}) Read the number of rows and columns in the table within CFITSIO's @code{fitsptr}. @end deftypefun @deftypefun int gal_fits_tab_format (fitsfile @code{*fitsptr}) Return the format of the FITS table contained in CFITSIO's @code{fitsptr}. Recall that FITS tables can be in binary or ASCII formats. This function will return @code{GAL_TABLE_FORMAT_AFITS} or @code{GAL_TABLE_FORMAT_BFITS} (defined in @ref{Table input output}). If the @code{fitsptr} is not a table, this function will abort the program with an error message informing the user of the problem. @end deftypefun @deftypefun {gal_data_t *} gal_fits_tab_info (char @code{*filename}, char @code{*hdu}, size_t @code{*numcols}, size_t @code{*numrows}, int @code{*tableformat}) Store the information of each column in @code{hdu} of @code{filename} into an array of data structures with @code{numcols} elements (one data structure for each column) see @ref{Arrays of datasets}. The total number of rows in the table is also put into the memory that @code{numrows} points to. The format of the table (e.g., FITS binary or ASCII table) will be put in @code{tableformat} (macros defined in @ref{Table input output}). This function is just for column information. Therefore it only stores meta-data like column name, units and comments. No actual data (contents of the columns for example the @code{array} or @code{dsize} elements) will be allocated by this function. This is a low-level function particular to reading tables in FITS format. To be generic, it is recommended to use @code{gal_table_info} which will allow getting information from a variety of table formats based on the filename (see @ref{Table input output}). @end deftypefun @deftypefun {gal_data_t *} gal_fits_tab_read (char @code{*filename}, char @code{*hdu}, size_t @code{numrows}, gal_data_t @code{*colinfo}, gal_list_sizet_t @code{*indexll}, int @code{minmapsize}) Read the columns given in the list @code{indexll} from a FITS table into a linked list of data structures, see @ref{List of size_t} and @ref{List of gal_data_t}. If the necessary space for each column is larger than @code{minmapsize}, don't keep it in the RAM, but in a file in the HDD/SSD, see the description under the same name in @ref{Generic data container}. Note that this is a low-level function, so the output data linked list is the inverse of the input indexs linked list. It is recommended to use @code{gal_table_read} for generic reading of tables, see @ref{Table input output}. @end deftypefun @deftypefun void gal_fits_tab_write (gal_data_t @code{*cols}, gal_list_str_t @code{*comments}, int @code{tableformat}, char @code{*filename}) Write the list of datasets in @code{cols} (see @ref{List of gal_data_t}) as separate columns in a FITS table in @code{filename}. If @code{filename} already exists then this function will write the table as a new extension after all existing ones. The format of the table (ASCII or binary) may be specified with the @code{tableformat} (see @ref{Table input output}). If @code{comments!=NULL}, each node of the list of strings will be written as a @code{COMMENT} keywords in the output FITS file (see @ref{List of strings}. This is a low-level function for tables. It is recommended to use @code{gal_table_write} for generic writing of tables in a variety of formats, see @ref{Table input output}. @end deftypefun @node World Coordinate System, Text files, FITS files, Gnuastro library @subsection World Coordinate System (@file{wcs.h}) The FITS standard defines the world coordinate system (WCS) as a mechanism to associate physical values to positions within a dataset. For example, it can be used to convert pixel coordinates in an image to celestial coordinates like the right ascension and declination. The functions in this section are mainly just wrappers over CFITSIO, WCSLIB and GSL library functions to help in common applications. @deftypefun {struct wcsprm *} gal_wcs_read_fitsptr (fitsfile @code{*fptr}, size_t @code{hstartwcs}, size_t @code{hendwcs}, int @code{*nwcs}) [@strong{Not thread-safe}] Return the WCSLIB @code{wcsprm} structure that is read from the CFITSIO @code{fptr} pointer to an opened FITS file. Also put the number of coordinate representations found into the space that @code{nwcs} points to. To read the WCS structure directly from a filename, see @code{gal_wcs_read} below. After processing has finished, you can free the returned structure with WCSLIB's @code{wcsvfree} keyword: @example status = wcsvfree(&nwcs,&wcs); @end example If you don't want to search the full FITS header for WCS-related FITS keywords (for example due to conflicting keywords), but only a specific range of the header keywords you can use the @code{hstartwcs} and @code{hendwcs} arguments to specify the keyword number range (counting from zero). If @code{hendwcs} is larger than @code{hstartwcs}, then only keywords in the given range will be checked. Hence, to ignore this feature (and search the full FITS header), give both these arguments the same value. If the WCS information couldn't be read from the FITS file, this function will return a @code{NULL} pointer and put a zero in @code{nwcs}. A WCSLIB error message will also be printed in @code{stderr} if there was an error. This function is just a wrapper over WCSLIB's @code{wcspih} function which is not thread-safe. Therefore, be sure to not call this function simultaneously (over multiple threads). @end deftypefun @deftypefun {struct wcsprm *} gal_wcs_read (char @code{*filename}, char @code{*hdu}, size_t @code{hstartwcs}, size_t @code{hendwcs}, int @code{*nwcs}) [@strong{Not thread-safe}] Return the WCSLIB structure that is read from the HDU/extension @code{hdu} of the file @code{filename}. Also put the number of coordinate representations found into the space that @code{nwcs} points to. Please see @code{gal_wcs_read_fitsptr} for more. @end deftypefun @deftypefun {struct wcsprm *} gal_wcs_copy (struct wcsprm @code{*wcs}) Return a fully allocated (independent) copy of @code{wcs}. @end deftypefun @deftypefun void gal_wcs_on_tile (gal_data_t @code{*tile}) Create a WCSLIB @code{wcsprm} structure for @code{tile} using WCS parameters of the tile's allocated block dataset, see @ref{Tessellation library} for the definition of tiles. If @code{tile} already has a WCS structure, this function won't do anything. In many cases, tiles are created for internal/low-level processing. Hence for performance reasons, when creating the tiles they don't have any WCS structure. When needed, this function can be used to add a WCS structure to each tile tile by copying the WCS structure of its block and correcting the reference point's coordinates within the tile. @end deftypefun @deftypefun {double *} gal_wcs_warp_matrix (struct wcsprm @code{*wcs}) Return the Warping matrix of the given WCS structure as an array of double precision floating points. This will be the final matrix, irrespective of the type of storage in the WCS structure. Recall that the FITS standard has several methods to store the matrix. The output is an allocated square matrix with each side equal to the number of dimensions. @end deftypefun @deftypefun void gal_wcs_decompose_pc_cdelt (struct wcsprm @code{*wcs}) Decompose the @code{PCi_j} and @code{CDELTi} elements of @code{wcs}. According to the FITS standard, in the @code{PCi_j} WCS formalism, the rotation matrix elements @mymath{m_{ij}} are encoded in the @code{PCi_j} keywords and the scale factors are encoded in the @code{CDELTi} keywords. There is also another formalism (the @code{CDi_j} formalism) which merges the two into one matrix. However, WCSLIB's internal operations are apparently done in the @code{PCi_j} formalism. So its outputs are also all in that format by default. When the input is a @code{CDi_j}, WCSLIB will still read the matrix directly into the @code{PCi_j} matrix and the @code{CDELTi} values are set to @code{1} (one). This function is designed to correct such issues: after it is finished, the @code{CDELTi} values in @code{wcs} will correspond to the pixel scale, and the @code{PCi_j} will correction show the rotation. @end deftypefun @deftypefun double gal_wcs_angular_distance_deg (double @code{r1}, double @code{d1}, double @code{r2}, double @code{d2}) Return the angular distance (in degrees) between a point located at (@code{r1}, @code{d1}) to (@code{r2}, @code{d2}). All input coordinates are in degrees. The distance (along a great circle) on a sphere between two points is calculated with the equation below. @dispmath {\cos(d)=\sin(d_1)\sin(d_2)+\cos(d_1)\cos(d_2)\cos(r_1-r_2)} However, since the the pixel scales are usually very small numbers, this function won't use that direct formula. It will be use the @url{https://en.wikipedia.org/wiki/Haversine_formula, Haversine formula} which is better considering floating point errors: @dispmath{{\sin^2(d)\over 2}=\sin^2\left( {d_1-d_2\over 2} \right)+\cos(d_1)\cos(d_2)\sin^2\left( {r_1-r_2\over 2} \right)} @end deftypefun @deftypefun {double *} gal_wcs_pixel_scale (struct wcsprm @code{*wcs}) Return the pixel scale for each dimension of @code{wcs} in degrees. The output is an array of double precision floating point type with one element for each dimension. @end deftypefun @deftypefun double gal_wcs_pixel_area_arcsec2 (struct wcsprm @code{*wcs}) Return the pixel area of @code{wcs} in arcsecond squared. If the input WCS structure is not two dimensional and the units (@code{CUNIT} keywords) are not @code{deg} (for degrees), then this function will return a NaN. @end deftypefun @deftypefun {gal_data_t *} gal_wcs_world_to_img (gal_data_t @code{*coords}, struct wcsprm @code{*wcs}, int @code{inplace}) Convert the linked list of world coordinates in @code{coords} to a linked list of image coordinates given the input WCS structure. @code{coords} must be a linked list of data structures of float64 (`double') type, see@ref{Linked lists} and @ref{List of gal_data_t}. The top (first popped/read) node of the linked list must be the first WCS coordinate (RA in an image usually) and etc. Similarly, the top node of the output will be the first image coordinate (in the FITS standard). If @code{inplace} is zero, then the output will be a newly allocated list and the input list will be untouched. However, if @code{inplace} is non-zero, the output values will be written into the input's already allocated array and the returned pointer will be the same pointer to @code{coords} (in other words, you can ignore the returned value). Note that in the latter case, only the values will be changed, things like units or name (if present) will be untouched. @end deftypefun @deftypefun {gal_data_t *} gal_wcs_img_to_world (gal_data_t @code{*coords}, struct wcsprm @code{*wcs}, int @code{inplace}) Convert the linked list of image coordinates in @code{coords} to a linked list of world coordinates given the input WCS structure. See the description of @code{gal_wcs_world_to_img} for more details. @end deftypefun @node Text files, Table input output, World Coordinate System, Gnuastro library @subsection Text files (@file{txt.h}) FITS files are the primary data container in astronomy. FITS indeed as many useful features, but the most universal and portable format for data storage are plain text files. They can be viewed and edited on any text editor or even on the command-line. Therefore the functions in this section are defined to simplify reading from and writing to plain text files. Lines are one of the most basic buiding blocks (delimiters) of a text file. Some operating systems like Microsoft Windows, terminate their ASCII text lines with a carriage return character and a new-line character (two characters, also known as CRLF line terminators). While Unix-like operating systems just use a single new-line character. The functions below that read an ASCII text file are able to identify lines with both kinds of line terminators. Gnuastro defines a simple format for metadata of table columns in a plain text file that is discussed in @ref{Gnuastro text table format}. The functions to get information from, read from and write to plain text files also follow those conventions. @deffn Macro GAL_TXT_LINESTAT_INVALID @deffnx Macro GAL_TXT_LINESTAT_BLANK @deffnx Macro GAL_TXT_LINESTAT_COMMENT @deffnx Macro GAL_TXT_LINESTAT_DATAROW Status codes for lines in a plain text file that are returned by @code{gal_txt_line_stat}. Lines which have a @key{#} character as their first non-white character are considered to be comments. Lines with nothing but white space characters are considered blank. The remaining lines are considered as containing data. @end deffn @deftypefun int gal_txt_line_stat (char @code{*line}) Check the contents of @code{line} and see if it is a blank, comment, or data line. The returned values are the macros that start with @code{GAL_TXT_LINESTAT}. @end deftypefun @deftypefun {gal_data_t *} gal_txt_table_info (char @code{*filename}, size_t @code{*numcols}, size_t @code{*numrows}) Store the information of each column in @code{filename} into an array of data structures with @code{numcols} elements (one data structure for each column) see @ref{Arrays of datasets}. The total number of rows in the table is also put into the memory that @code{numrows} points to. This function is just for column information. Therefore it only stores meta-data like column name, units and comments. No actual data (contents of the columns for example the @code{array} or @code{dsize} elements) will be allocated by this function. This is a low-level function particular to reading tables in plain text format. To be generic, it is recommended to use @code{gal_table_info} which will allow getting information from a variety of table formats based on the filename (see @ref{Table input output}). @end deftypefun @deftypefun {gal_data_t *} gal_txt_table_read (char @code{*filename}, size_t @code{numrows}, gal_data_t @code{*colinfo}, gal_list_sizet_t @code{*indexll}, size_t @code{minmapsize}) Read the columns given in the list @code{indexll} from a plain text table into a linked list of data structures, see @ref{List of size_t} and @ref{List of gal_data_t}. If the necessary space for each column is larger than @code{minmapsize}, don't keep it in the RAM, but in a file on the HDD/SSD, see the description under the same name in @ref{Generic data container}. Note that this is a low-level function, so the output data list is the inverse of the input indexs linked list. It is recommended to use @code{gal_table_read} for generic reading of tables in any format, see @ref{Table input output}. @end deftypefun @deftypefun {gal_data_t *} gal_txt_image_read (char @code{*filename}, size_t @code{minmapsize}) Read the 2D plain text dataset in @code{filename} into a dataset and return the dataset. If the necessary space for the image is larger than @code{minmapsize}, don't keep it in the RAM, but in a file on the HDD/SSD, see the description under the same name in @ref{Generic data container}. @end deftypefun @deftypefun void gal_txt_write (gal_data_t @code{*cols}, gal_list_str_t @code{*comment}, char @code{*filename}) Write @code{cols} in a plain text file @code{filename}. @code{cols} may have one or two dimensions which determines the output: @table @asis @item 1D @code{cols} is treated as a column and a list of datasets (see @ref{List of gal_data_t}): every node in the list is written as one column in a table. @item 2D @code{cols} is a two dimensional array, it cannot be treated as a list (only one 2D array can currently be written to a text file). So if @code{cols->next!=NULL} the next nodes in the list are ignored and will not be written. @end table If @code{filename} already exists this function will abort with an error and will not write over the existing file. Please make sure if the file exists or not and take the appropriate action before calling this function. If @code{comments!=NULL}, a @code{#} will be put at the start of each node of the list of strings and will be written in the file before the column meta-data in @code{filename} (see @ref{List of strings}). This is a low-level function for tables. It is recommended to use @code{gal_table_write} for generic writing of tables in a variety of formats, see @ref{Table input output}. @end deftypefun @node Table input output, Arithmetic on datasets, Text files, Gnuastro library @subsection Table input output (@file{table.h}) Tables are a collection of one dimensional datasets that are packed together into one file. They are the single most common format to store high-level (processed) information, hence they play a very important role in Gnuastro. For a more thorough introduction, please see @ref{Table}. Gnuastro's Table program, and all the other programs that can read from and write into tables, use the functions of this section for reading and writing their input/output tables. For a simple demonstration of using the constructs introduced here, see @ref{Library demo - reading and writing table columns}. Currently only plain text (see @ref{Gnuastro text table format}) and FITS (ASCII and binary) tables are supported by Gnuastro. However, the low-level table infra-structure is written such that accommodating other formats is also possible and in future releases more formats will hopefully be supported. Please don't hesitate to suggest your favorite format so it can be implemented when possible. @deffn Macro GAL_TABLE_DEF_WIDTH_STR @deffnx Macro GAL_TABLE_DEF_WIDTH_INT @deffnx Macro GAL_TABLE_DEF_WIDTH_LINT @deffnx Macro GAL_TABLE_DEF_WIDTH_FLT @deffnx Macro GAL_TABLE_DEF_WIDTH_DBL @deffnx Macro GAL_TABLE_DEF_PRECISION_INT @deffnx Macro GAL_TABLE_DEF_PRECISION_FLT @deffnx Macro GAL_TABLE_DEF_PRECISION_DBL @cindex @code{printf} The default width and precision for generic types to use in writing numeric types into a text file (plain text and FITS ASCII tables). When the dataset doesn't have any pre-set width and precision (see @code{disp_width} and @code{disp_precision} in @ref{Generic data container}) these will be directly used in C's @code{printf} command to write the number as a string. @end deffn @deffn Macro GAL_TABLE_DISPLAY_FMT_STRING @deffnx Macro GAL_TABLE_DISPLAY_FMT_DECIMAL @deffnx Macro GAL_TABLE_DISPLAY_FMT_UDECIMAL @deffnx Macro GAL_TABLE_DISPLAY_FMT_OCTAL @deffnx Macro GAL_TABLE_DISPLAY_FMT_HEX @deffnx Macro GAL_TABLE_DISPLAY_FMT_FLOAT @deffnx Macro GAL_TABLE_DISPLAY_FMT_EXP @deffnx Macro GAL_TABLE_DISPLAY_FMT_GENERAL The display format used in C's @code{printf} to display data of different types. The @code{_STRING} and @code{_DECIMAL} are unique for printing strings and signed integers, they are mainly here for completeness. However, unsigned integers and floating points can be displayed in multiple formats: @table @asis @item Unsigned integer For unsigned integers, it is possible to choose from @code{_UDECIMAL} (unsigned decimal), @code{_OCTAL} (octal notation, for example @code{125} in decimal will be displayed as @code{175}), and @code{_HEX} (hexadecimal notation, for example @code{125} in decimal will be displayed as @code{7D}). @item Floating point For floating point, it is possible to display the number in @code{_FLOAT} (floating point, for example @code{1500.345}), @code{_EXP} (exponential, for example @code{1.500345e+03}), or @code{_GENERAL} which is the best of the two for the given number. @end table @end deffn @deffn Macro GAL_TABLE_FORMAT_INVALID @deffnx Macro GAL_TABLE_FORMAT_TXT @deffnx Macro GAL_TABLE_FORMAT_AFITS @deffnx Macro GAL_TABLE_FORMAT_BFITS All the current acceptable table formats to Gnuastro. The @code{AFITS} and @code{BFITS} represent FITS ASCII tables and FITS Binary tables. You can use these anywhere you see the @code{tableformat} variable. @end deffn @deffn Macro GAL_TABLE_SEARCH_INVALID @deffnx Macro GAL_TABLE_SEARCH_NAME @deffnx Macro GAL_TABLE_SEARCH_UNIT @deffnx Macro GAL_TABLE_SEARCH_COMMENT When the desired column is not a number, these values determine if the string to match, or regular expression to search, be in the @emph{name}, @emph{units} or @emph{comments} of the column meta data. These values should be used for the @code{searchin} variables of the functions. @end deffn @deftypefun {gal_data_t *} gal_table_info (char @code{*filename}, char @code{*hdu}, size_t @code{*numcols}, size_t @code{*numrows}, int @code{*tableformat}) Store the information of each column in a table (either as a text file or as a FITS table) into an array of data structures with @code{numcols} structures (one data structure for each column). The number of rows is stored in the space that @code{numrows} points to. The format of the table (e.g., ascii text file, or FITS binary or ASCII table) will be put in @code{tableformat} (macros defined above). If the filename is not a FITS file, then @code{hdu} will not be used (can be @code{NULL}). Note that other than the character strings (column name, units and comments), nothing in the data structure(s) will be allocated by this function for the actual data (e.g., the `array' or `dsize' elements). This function is just for column information (meta-data), not column contents. @end deftypefun @deftypefun void gal_table_print_info (gal_data_t @code{*allcols}, size_t @code{numcols}, size_t @code{numrows}) This program will print the column information for all the columns (output of @code{gal_table_info}). The output is in the same format as this command with Gnuastro Table program (see @ref{Table}): @example $ asttable --info table.fits @end example @end deftypefun @deftypefun {gal_data_t *} gal_table_read (char @code{*filename}, char @code{*hdu}, gal_list_str_t @code{*cols}, int @code{searchin}, int @code{ignorecase}, int @code{minmapsize}, size_t @code{colmatch}) Read the specified columns in a text file (named @code{filename}) into a linked list of data structures. If the file is FITS, then @code{hdu} will also be used, otherwise, @code{hdu} is ignored. @cindex AWK @cindex GNU AWK The information to search for columns should be specified by the @code{cols} list of strings (see @ref{List of strings}). The string in each node of the list may be a number, an exact match to a column name, or a regular expression (in GNU AWK format) enclosed in @code{/ /}. The @code{searchin} value must be one of the macros defined above. If @code{cols} is NULL, then this function will read the full table. The output is an individually allocated list of datasets (see @ref{List of gal_data_t}) with the same order of the @code{cols} list. Note that one column node in the @code{cols} list might give multiple columns (for example from regular expressions), in this case, the order of output columns that correspond to that one input, are in order of the table (which column was read first). So the first requested column is the first popped data structure and so on. if @code{colmatch!=NULL}, it is assumed to be an array that has at least the same number of elements as nodes in the @code{cols} list. The number of columns that matched each input column will be stored in each element. @end deftypefun @cindex Git @deftypefun void gal_table_comments_add_intro (gal_list_str_t @code{**comments}, char @code{*program_string}, time_t @code{*rawtime}) Add some basic information to the list of @code{comments}. This basic information includes the following information @itemize @item If the program is run in a Git version controlled directory, Git's description is printed (see description under @code{COMMIT} in @ref{Output headers}). @item The calendar time that is stored in @code{rawtime} (@code{time_t} is C's calendar time format defined in @file{time.h}). You can calculate the time in this format with the following expressions: @example time_t rawtime; time(&rawtime); @end example @item The name of your program in @code{program_string}. If it is @code{NULL}, this line is ignored. @end itemize @end deftypefun @deftypefun void gal_table_write (gal_data_t @code{*cols}, gal_list_str_t @code{*comments}, int @code{tableformat}, char @code{*filename}, char @code{*extname}) Write the @code{cols} list of datasets into a table in @code{filename} (see @ref{List of gal_data_t}). The format of the table can be determined with @code{tableformat} that accepts the macros defined above. If @code{comments} is not @code{NULL}, then the list of comments will also be printed into the output table. When the output table is a plain text file, each node's string will be printed after a @code{#} (so it can be considered as a comment) and in FITS table they will follow a @code{COMMENT} keyword. If @file{filename} is a FITS file, the table extension that will be written will have the name @code{extname}. If a file named @file{filename} already exists, the operation depends on the type of output. When @file{filename} is a FITS file, the table will be added as a new extension after all existing ones. If @file{filename} is a plain text file, this function will abort with an error. @end deftypefun @deftypefun void gal_table_write_log (gal_data_t @code{*logll}, char @code{*program_string}, time_t @code{*rawtime}, gal_list_str_t @code{*comments}, char @code{*filename}, int @code{quiet}) Write the @code{logll} list of datasets into a table in @code{filename} (see @ref{List of gal_data_t}). This function is just a wrapper around @code{gal_table_comments_add_intro} and @code{gal_table_write} (see above). If @code{quiet} is non-zero, this function will print a message saying that the @code{filename} has been created. @end deftypefun @node Arithmetic on datasets, Tessellation library, Table input output, Gnuastro library @subsection Arithmetic on datasets (@file{arithmetic.h}) When the dataset's type and other information are already known, any programming language (including C) provides some very good tools for various operations (including arithmetic operations like addition) on the dataset with a simple loop. However, as an author of a program, making assumptions about the type of data, its dimensions and other basic characteristics will come with a large processing burden. For example if you always read your data as double precision floating points for a simple operation like addition with an integer constant, you will be wasting a lot of CPU and memory when the input dataset is @code{int32} type for example (see @ref{Numeric data types}). This overhead may be small for small images, but as you scale your process up and work with hundred/thousands of files that can be very large, this overhead will take a significant portion of the processing power. The functions and macros in this section are designed precisely for this purpose: to allow you to do any of the defined operations on any dataset with no overhead (in the native type of the dataset). Gnuastro's Arithmetic program uses the functions and macros of this section, so please also have a look at the @ref{Arithmetic} program and in particular @ref{Arithmetic operators} for a better description of the operators discussed here. The main function of this library is @code{gal_arithmetic} that is described below. It can take an arbitrary number of arguments as operands (depending on the operator, similar to @code{printf}). Its first two arguments are integers specifying the flags and operator. So first we will review the constants for the recognized flags and operators and discuss them, then introduce the actual function. @deffn Macro GAL_ARITHMETIC_INPLACE @deffnx Macro GAL_ARITHMETIC_FREE @deffnx Macro GAL_ARITHMETIC_NUMOK @deffnx Macro GAL_ARITHMETIC_FLAGS_ALL @cindex Bitwise Or Bit-wise flags to pass onto @code{gal_arithmetic} (see below). To pass multiple flags, use the bitwise-or operator, for example @code{GAL_ARITHMETIC_INPLACE | GAL_ARITHMETIC_FREE}. @code{GAL_ARITHMETIC_FLAGS_ALL} is a combination of all flags to shorten your code if you want all flags activated. Each flag is described below: @table @code @item GAL_ARITHMETIC_INPLACE Do the operation in-place (in the input dataset, thus modifying it) to improve CPU and memory usage. If this flag is used, after @code{gal_arithmetic} finishes, the input dataset will be modified. It is thus useful if you have no more need for the input after the operation. @item GAL_ARITHMETIC_FREE Free (all the) input dataset(s) after the operation is done. Hence the inputs are no longer usable after @code{gal_arithmetic}. @item GAL_ARITHMETIC_NUMOK It is acceptable to use a number and an array together. For example if you want to add all the pixels in an image with a single number you can pass this flag to avoid having to allocate a constant array the size of the image (with all the pixels having the same number). @end table @end deffn @deffn Macro GAL_ARITHMETIC_OP_PLUS @deffnx Macro GAL_ARITHMETIC_OP_MINUS @deffnx Macro GAL_ARITHMETIC_OP_MULTIPLY @deffnx Macro GAL_ARITHMETIC_OP_DIVIDE @deffnx Macro GAL_ARITHMETIC_OP_LT @deffnx Macro GAL_ARITHMETIC_OP_LE @deffnx Macro GAL_ARITHMETIC_OP_GT @deffnx Macro GAL_ARITHMETIC_OP_GE @deffnx Macro GAL_ARITHMETIC_OP_EQ @deffnx Macro GAL_ARITHMETIC_OP_NE @deffnx Macro GAL_ARITHMETIC_OP_AND @deffnx Macro GAL_ARITHMETIC_OP_OR Binary operators (requiring two operands) that accept datasets of any recognized type (see @ref{Numeric data types}). When @code{gal_arithmetic} is called with any of these operators, it expects two datasets as arguments. For a full description of these operators with the same name, see @ref{Arithmetic operators}. The first dataset/operand will be put on the left of the operator and the second will be put on the right. The output type of the first four is determined from the input types (largest type of the inputs). The rest (which are all conditional operators) will output a binary @code{uint8_t} (or @code{unsigned char}) dataset with values of either @code{0} (zero) or @code{1} (one). @end deffn @deffn Macro GAL_ARITHMETIC_OP_NOT The logical NOT operator. When @code{gal_arithmetic} is called with this operator, it only expects one operand (dataset), since this is a unary operator. The output is @code{uint8_t} (or @code{unsigned char}) dataset of the same size as the input. Any non-zero element in the input will be @code{0} (zero) in the output and any @code{0} (zero) will have a value of @code{1} (one). @end deffn @deffn Macro GAL_ARITHMETIC_OP_ISBLANK A unary operator with output that is @code{1} for any element in the input that is blank, and @code{0} for any non-blank element. When @code{gal_arithmetic} is called with this operator, it will only expect one input dataset. The output dataset will have @code{uint8_t} (or @code{unsigned char}) type. @code{gal_arithmetic} with this operator is just a wrapper for the @code{gal_blank_flag} function of @ref{Library blank values} and this operator is just included for completeness in arithmetic operations. So in your program, it might be easier to just call @code{gal_blank_flag}. @end deffn @deffn Macro GAL_ARITHMETIC_OP_WHERE The three-operand @emph{where} operator thoroughly discussed in @ref{Arithmetic operators}. When @code{gal_arithmetic} is called with this operator, it will only expect three input datasets: the first (which is the same as the returned dataset) is the array that will be modified. The second is the condition dataset (that must have a @code{uint8_t} or @code{unsigned char} type), and the third is the value to be used if condition is non-zero. As a result, note that the order of operands when calling @code{gal_arithmetic} with @code{GAL_ARITHMETIC_OP_WHERE} is the opposite of running Gnuastro's Arithmetic program with the @code{where} operator (see @ref{Arithmetic}). This is because the latter uses the reverse-Polish notation which isn't necessary when calling a function (see @ref{Reverse polish notation}). @end deffn @deffn Macro GAL_ARITHMETIC_OP_SQRT @deffnx Macro GAL_ARITHMETIC_OP_LOG @deffnx Macro GAL_ARITHMETIC_OP_LOG10 Unary operator functions for calculating the square root (@mymath{\sqrt{i}}), @mymath{ln(i)} and @mymath{log(i)} mathematic operators on each element of the input dataset. The output will have the same type as the input, so if your inputs are integer types be careful. If you want your output to be floating point but your input is an integer type, you can convert the input to a floating point type with @code{gal_data_copy_to_new_type} or @code{gal_data_copy_to_new_type_free}(see @ref{Copying datasets}). @end deffn @deffn Macro GAL_ARITHMETIC_OP_MINVAL @deffnx Macro GAL_ARITHMETIC_OP_MAXVAL @deffnx Macro GAL_ARITHMETIC_OP_NUMVAL @deffnx Macro GAL_ARITHMETIC_OP_SUMVAL @deffnx Macro GAL_ARITHMETIC_OP_MEANVAL @deffnx Macro GAL_ARITHMETIC_OP_STDVAL @deffnx Macro GAL_ARITHMETIC_OP_MEDIANVAL Unary operand statistical operators that will return a single value for datasets of any size. These are just wrappers around similar functions in @ref{Statistical operations} and are included in @code{gal_arithmetic} only for completeness (to use easily in @ref{Arithmetic}). In your programs, it will probably be easier if you use those @code{gal_statistics_} functions directly. @end deffn @deffn Macro GAL_ARITHMETIC_OP_ABS Unary operand absolute-value operator. @end deffn @deffn Macro GAL_ARITHMETIC_OP_MIN @deffnx Macro GAL_ARITHMETIC_OP_MAX @deffnx Macro GAL_ARITHMETIC_OP_NUM @deffnx Macro GAL_ARITHMETIC_OP_SUM @deffnx Macro GAL_ARITHMETIC_OP_MEAN @deffnx Macro GAL_ARITHMETIC_OP_STD @deffnx Macro GAL_ARITHMETIC_OP_MEDIAN Multi-operand statistical operations. When @code{gal_arithmetic} is called with any of these operators, it will expect only a single operand that will be interpretted as a list of datasets (see @ref{List of gal_data_t}. The output will be a single dataset with each of its elements replaced by the respective statistical operation on the whole list. See the discussion under the @code{min} operator in @ref{Arithmetic operators}. @end deffn @deffn Macro GAL_ARITHMETIC_OP_POW Binary operator to-power operator. When @code{gal_arithmetic} is called with any of these operators, it will expect two operands: raising the first by the second. This operator only accepts floating point inputs and the output is also floating point. @end deffn @deffn Macro GAL_ARITHMETIC_OP_BITAND @deffnx Macro GAL_ARITHMETIC_OP_BITOR @deffnx Macro GAL_ARITHMETIC_OP_BITXOR @deffnx Macro GAL_ARITHMETIC_OP_BITLSH @deffnx Macro GAL_ARITHMETIC_OP_BITRSH @deffnx Macro GAL_ARITHMETIC_OP_MODULO Binary integer-only operand operators. These operators are only defined on integer data types. When @code{gal_arithmetic} is called with any of these operators, it will expect two operands: the first is put on the left of the operator and the second on the right. The ones starting with @code{BIT} are the respective bit-wise operators in C and @code{MODULO} is the modulo/remainder operator. For a discussion on these operators, please see @ref{Arithmetic operators}. The output type is determined from the input types and C's internal conversions: it is strongly recommended that both inputs have the same type (any integer type), otherwise the bit-wise behavior will be determined by your compiler. @end deffn @deffn Macro GAL_ARITHMETIC_OP_BITNOT The unary bit-wise NOT operator. When @code{gal_arithmetic} is called with any of these operators, it will expect one operand of an integer type and preform the bitwise-NOT operation on it. The output will have the same type as the input. @end deffn @deffn Macro GAL_ARITHMETIC_OP_TO_UINT8 @deffnx Macro GAL_ARITHMETIC_OP_TO_INT8 @deffnx Macro GAL_ARITHMETIC_OP_TO_UINT16 @deffnx Macro GAL_ARITHMETIC_OP_TO_INT16 @deffnx Macro GAL_ARITHMETIC_OP_TO_UINT32 @deffnx Macro GAL_ARITHMETIC_OP_TO_INT32 @deffnx Macro GAL_ARITHMETIC_OP_TO_UINT64 @deffnx Macro GAL_ARITHMETIC_OP_TO_INT64 @deffnx Macro GAL_ARITHMETIC_OP_TO_FLOAT32 @deffnx Macro GAL_ARITHMETIC_OP_TO_FLOAT64 Unary type-conversion operators. When @code{gal_arithmetic} is called with any of these operators, it will expect one operand and convert it to the requested type. Note that with these operators, @code{gal_arithmetic} is just a wrapper over the @code{gal_data_copy_to_new_type} or @code{gal_data_copy_to_new_type_free} that are discussed in @code{Copying datasets}. It accepts these operators only for completeness and easy usage in @ref{Arithmetic}. So in your programs, it might be preferable to directly use those functions. @end deffn @deftypefun {gal_data_t *} gal_arithmetic (int operator, int flags, ...) Do the arithmetic operation of @code{operator} on the given operands (the third argument and any further argument). Certain special conditions can also be specified with the @code{flag} operator. The acceptable values for @code{operator} are defined in the macros above. @code{gal_arithmetic} is a multi-argument function (like C's @code{printf}). In other words, the number of necessary arguments is not fixed and depends on the value to @code{operator}. Here are a few examples showing this variability: @example out_1=gal_arithmetic(GAL_ARITHMETIC_OP_LOG, 0, in_1); out_2=gal_arithmetic(GAL_ARITHMETIC_OP_PLUS, 0, in_1, in_2); out_3=gal_arithmetic(GAL_ARITHMETIC_OP_WHERE, 0, in_1, in_2, in_3); @end example The number of necessary operands for each operator (and thus the number of necessary arguments to @code{gal_arithmetic}) are described above under each operator. @end deftypefun @node Tessellation library, Bounding box, Arithmetic on datasets, Gnuastro library @subsection Tessellation library (@file{tile.h}) In many contexts, it is desirable to slice the dataset into subsets or tiles (overlapping or not). In such a way that you can work on each tile independently. One method would be to copy that region to a separate allocated space, but in many contexts this isn't necessary and in fact can be a big burden on CPU/Memory usage. The @code{block} pointer in Gnuastro's @ref{Generic data container} is defined for such situations: where allocation is not necessary. You just want to read the data or write to it independently (or in coordination with) other regions of the dataset. Added with parallel processing, this can greatly improve the time/memory consumption. See the figure below for example: assume the @code{larger} dataset is a contiguous block of memory that you are interpreting as a 2D array. But you only want to work on the smaller @code{tile} region. @example larger --------------------------------- | | | tile | | ---------- | | | | | | |_ | | | |*| | | | ---------- | | tile->block = larger | |_ | |*| | --------------------------------- @end example To use @code{gal_data_t}'s @code{block} concept, you allocate a @code{gal_data_t *tile} which is initialized with the pointer to the first element in the sub-array (as its @code{array} argument). Note that this is not necessarily the first element in the larger array. You can set the size of the tile along with the initialization as you please. Recall that, when given a non-@code{NULL} pointer as @code{array}, @code{gal_data_initialize} (and thus @code{gal_data_alloc}) do not allocate any space and just uses the given pointer for the new @code{array} element of the @code{gal_data_t}. So your @code{tile} data structure will not be pointing to a separately allocated space. After the allocation is done, you just point @code{tile->block} to the @code{larger} dataset which hosts the full block of memory. Where relevant, Gnuastro's library functions will check the @code{block} pointer of their input dataset to see how to deal with dimensions and increments so they can always remain within the tile. The tools introduced in this section are designed to help in defining and working with tiles that are created in this manner. Since the block structure is defined as a pointer, arbitrary levels of tessellation/grid-ing are possible (@code{tile->block} may itself be a tile in an even larger allocated space). Therefore, just like a linked-list (see @ref{Linked lists}), it is important to have the @code{block} pointer of the largest (allocated) dataset set to @code{NULL}. Normally, you won't have to worry about this, because @code{gal_data_initialize} (and thus @code{gal_data_alloc}) will set the @code{block} element to @code{NULL} by default, just remember not to change it. You can then only change the @code{block} element for the tiles you define over the allocated space. Below, we will first review constructs for @ref{Independent tiles} and then define the current approach to fully tessellating a dataset (or covering every pixel/data-element with a non-overlapping tile grid in @ref{Tile grid}. This approach to dealing with parts of a larger block was inspired from a similarly named concept in the GNU Scientific Library (GSL), see its ``Vectors and Matrices'' chapter for their implementation. @menu * Independent tiles:: Work on or check independent tiles. * Tile grid:: Cover a full dataset with non-overlapping tiles. @end menu @node Independent tiles, Tile grid, Tessellation library, Tessellation library @subsubsection Independent tiles The most general application of tiles is to treat each independently, for example they may overlap, or they may not cover the full image. This section provides functions to help in checking/inspecting such tiles. In @ref{Tile grid} we will discuss functions that define/work-with a tile grid (where the tiles don't overlap and fully cover the input dataset). Therefore, the functions in this section are general and can be used for the tiles produced by that section also. @deftypefun void gal_tile_start_coord (gal_data_t @code{*tile}, size_t @code{*start_coord}) Calculate the starting coordinates of a tile in its allocated block of memory and write them in the memory that @code{start_coord} points to (which must have @code{tile->ndim} elements). @end deftypefun @deftypefun void gal_tile_start_end_coord (gal_data_t @code{*tile}, size_t @code{*start_end}, int @code{rel_block}) Put the starting and ending (end point is not inclusive) coordinates of @code{tile} into the @code{start_end} array. It is assumed that a space of @code{2*tile->ndim} has been already allocated (static or dynamic) for @code{start_end} before this function is called. @code{rel_block} (or relative-to-block) is only relevant when @code{tile} has an intermediate tile between it and the allocated space (like a channel, see @code{gal_tile_full_two_layers}). If it doesn't (@code{tile->block} points the allocated dataset), then the value to @code{rel_block} is irrelevant. When @code{tile->block} is its self a larger block and @code{rel_block} is set to 0, then the starting and ending positions will be based on the position within @code{tile->block}, not the allocated space. @end deftypefun @deftypefun {void *} gal_tile_start_end_ind_inclusive (gal_data_t @code{*tile}, gal_data_t @code{*work}, size_t @code{*start_end_inc}) Put the indexs of the first/start and last/end pixels (inclusive) in a tile into the @code{start_end} array (that must have two elements). NOTE: this function stores the index of each point, not its coordinates. It will then return the pointer to the start of the tile in the @code{work} data structure (which doesn't have to be equal to @code{tile->block}. The outputs of this function are defined to make it easy to parse over an n-dimensional tile. For example, this function is one of the most important parts of the internal processing of in @code{GAL_TILE_PARSE_OPERATE} function-like macro that is described below. @end deftypefun @deftypefun {gal_data_t *} gal_tile_series_from_minmax (gal_data_t @code{*block}, size_t @code{*minmax}, size_t @code{number}) Construct a list of tile(s) given coordinates of the minimum and maximum of each tile. The minimum and maximums are assumed to be inclusive. The returned pointer is an allocated @code{gal_data_t} array that can later be freed with @code{gal_data_array_free} (see @ref{Arrays of datasets}). Internally, each element of the output array points to the next element, so the output may also be treated as a list of datasets (see @ref{List of gal_data_t}) and passed onto the other functions described in this section. The array keeping the minimum and maximum coordinates for each tile must have the following format. So in total @code{minmax} must have @code{2*ndim*number} elements. @example | min0_d0 | min0_d1 | max0_d0 | max0_d1 | ... ... | minN_d0 | minN_d1 | maxN_d0 | maxN_d1 | @end example @end deftypefun @deftypefun {gal_data_t *} gal_tile_block (gal_data_t @code{*tile}) Return the dataset that contains @code{tile}'s allocated block of memory. If tile is immediately defined as part of the allocated block, then this is equivalent to @code{tile->block}. However, it is possible to have multiple layers of tiles (where @code{tile->block} is itself a tile). So this function is the most generic way to get to the actual allocated dataset. @end deftypefun @deftypefun size_t gal_tile_block_increment (gal_data_t @code{*block}, size_t @code{*tsize}, size_t @code{num_increment}, size_t @code{*coord}) Return the increment necessary to start at the next contiguous patch memory associated with a tile. @code{block} is the allocated block of memory and @code{tsize} is the size of the tile along every dimension. If @code{coord} is @code{NULL}, it is ignored. Otherwise, it will contain the coordinate of the start of the next contiguous patch of memory. This function is intended to be used in a loop and @code{num_increment} is the main variable to this function. For the first time you call this function, it should be @code{1}. In subsequent calls (while you are parsing a tile), it should be increased by one. @end deftypefun @deftypefun {gal_data_t *} gal_tile_block_write_const_value (gal_data_t @code{*tilevalues}, gal_data_t @code{*tilesll}, int @code{withblank}, int @code{initialize}) Write a constant value for each tile over the area it covers in an allocated dataset that is the size of @code{tile}'s allocated block of memory (found through @code{gal_tile_block} described above). The arguments to this function are: @table @code @item tilevalues This must be an array that has the same number of elements as the nodes in in @code{tilesll} and in the same order that `tilesll' elements are parsed (from top to bottom, see @ref{Linked lists}). As a result the array's number of dimensions is irrelevant, it will be parsed contiguously. @item tilesll The list of input tiles (see @ref{List of gal_data_t}). Internally, it might be stored as an array (for example the output of @code{gal_tile_series_from_minmax} described above), but this function doesn't care, it will parse the @code{next} elements to go to the next tile. This function will not pop-from or free the @code{tilesll}, it will only parse it from start to end. @item withblank If the block containing the tiles has blank elements, those blank elements will be blank in the output of this function also, hence the array will be initialized with blank values when this option is called (see below). @item initialize Initialize the allocated space with blank values before writing in the constant values. This can be useful when the tiles don't cover the full allocated block. @end table @end deftypefun @deftypefun {gal_data_t *} gal_tile_block_check_tiles (gal_data_t @code{*tilesll}) Make a copy of the memory block and fill it with the index of each tile in @code{tilesll} (counting from 0). The non-filled areas will have blank values. The output dataset will have a type of @code{GAL_TYPE_INT32} (see @ref{Library data types}). This function can be used when you want to check the coverage of each tile over the allocated block of memory. It is just a wrapper over the @code{gal_tile_block_write_const_value} (with @code{withblank} set to zero). @end deftypefun @deftypefun {void *} gal_tile_block_relative_to_other (gal_data_t @code{*tile}, gal_data_t @code{*other}) Return the pointer corresponding to the start of the region covered by @code{tile} over the @code{other} dataset. See the examples in @code{GAL_TILE_PARSE_OPERATE} for some example applications of this function. @end deftypefun @deftypefun void gal_tile_block_blank_flag (gal_data_t @code{*tilell}, size_t @code{numthreads}) Check if each tile in the list has blank values and update its @code{flag} to mark this check and its result (see @ref{Generic data container}). The operation will be done on @code{numthreads} threads. @end deftypefun @deffn {Function-like macro} GAL_TILE_PARSE_OPERATE (@code{IN}, @code{OTHER}, @code{PARSE_OTHER}, @code{CHECK_BLANK}, @code{OP}) Parse @code{IN} (which can be a tile or a fully allocated block of memory) and do the @code{OP} operation on it. @code{OP} can be any combination of C expressions. If @code{OTHER!=NULL}, @code{OTHER} will be interpretted as a dataset and this macro will allow access to its element(s) and it can optionally be parsed while parsing over @code{IN}. If @code{OTHER} is a fully allocated block of memory (not a tile), then the same region that is covered by @code{IN} within its own block will be parsed (the same starting pixel with the same number of pixels in each dimension). Hence, in this case, the blocks of @code{OTHER} and @code{IN} must have the same size. When @code{OTHER} is a tile it must have the same size as @code{IN} and parsing will start from its starting element/pixel. Also, the respective allocated blocks of @code{OTHER} and @code{IN} (if different) may have different sizes. Using @code{OTHER} (along with @code{PARSE_OTHER}), this funciton-like macro will thus enable you to parse and define your own operation on two fixed size regions in one or two blocks of memory. In the latter case, they may have different numeric datatypes, see @ref{Numeric data types}). The input arguments to this macro are explained below, the expected type of each argument are also written following the argument name: @table @code @item IN (gal_data_t) Input dataset, this can be a tile or an allocated block of memory. @item OTHER (gal_data_t) Dataset (@code{gal_data_t}) to parse along with @code{IN}. It can be @code{NULL}. In that case, @code{o} (see description of @code{OP} below) will be @code{NULL} and should not be used. If @code{PARSE_OTHER} is zero, only its first element will be used and the size of this dataset is irrelevant. When @code{OTHER} is a block of memory, it has to have the same size as the allocated block of @code{IN}. When its a tile, it has to have the same size as @code{IN}. @item PARSE_OTHER (int) Parse the other dataset along with the input. When this is non-zero and @code{OTHER!=NULL}, then the @code{o} pointer will be incremented to cover the @code{OTHER} tile at the same rate as @code{i}, see description of @code{OP} for @code{i} and @code{o}. @item CHECK_BLANK (int) If it is non-zero, then the input will be checked for blank values and @code{OP} will only be called when we are not on a blank element. @item OP Operator: this can be any number of C expressions. This macro is going to define a @code{itype *i} variable which will increment over each element of the input array/tile. @code{itype} will be replaced with the C type that corresponds to the type of @code{INPUT}. As an example, if @code{INPUT}'s type is @code{GAL_DATA_UINT16} or @code{GAL_DATA_FLOAT32}, @code{i} will be defined as @code{uint16} or @code{float} respectively. This function-like macro will also define an @code{otype *o} which you can use to access an element of the @code{OTHER} dataset (if @code{OTHER!=NULL}). @code{o} will correspond to the type of @code{OTHER} (similar to @code{itype} and @code{INPUT} discussed above). If @code{PARSE_OTHER} is non-zero, then @code{o} will also be incremented to the same index element but in the other array. You can use these along with any other variable you define before this macro to process the input and store it in the other. All variables within this function-like macro begin with @code{tpo_} except for the three variables listed above. So as long as you don't start the names of your variables with this prefix everything will be fine. Note that @code{i} (and possibly @code{o}) will be incremented once by this function-like macro, so don't increment them within @code{OP}. As a summary, the three variables you have access to within @code{OP} are: @table @code @item i Pointer to the element of @code{INPUT} that is being parsed with the proper type. @item o Pointer to the element of @code{OTHER} that is being parsed with the proper type. @code{o} can only be used if @code{OTHER!=NULL} and it will be parsed/incremented if @code{PARSE_OTHER} is non-zero. @item b Blank value in the type of @code{INPUT}. @end table @end table You can use a given tile (@code{tile} on a dataset that it was not initialized with but has the same size, let's call it @code{new}) with the following steps: @example void *tarray; gal_data_t *tblock; /* `tile->block' must be corrected AFTER `tile->array'. */ tarray = tile->array; tblock = tile->block; tile->array = gal_tile_block_relative_to_other(tile, new); tile->block = new; /* Parse and operate over this region of the `new' dataset. */ GAL_TILE_PARSE_OPERATE(tile, NULL, 0, 0, @{ YOUR_PROCESSING; @}); /* Reset `tile->block' and `tile->array'. */ tile->array=tarray; tile->block=tblock; @end example You can work on the same region of another block in one run of this function-like macro. To do that, you can make a fake tile and pass that as the @code{OTHER} argument. Below is a demonstration, @code{tile} is the actual tile that you start with and @code{new} is the other block of allocated memory. @example size_t zero=0; gal_data_t *faketile; /* Allocate the fake tile, these can be done outside a loop * (over many tiles). */ faketile=gal_data_alloc(NULL, new->type, 1, &zero, NULL, 0, -1, NULL, NULL, NULL); free(faketile->array); /* To keep things clean. */ free(faketile->dsize); /* To keep things clean. */ faketile->block = new; faketile->ndim = new->ndim; /* These can be done in a loop (over many tiles). */ faketile->size = tile->size; faketile->dsize = tile->dsize; faketile->array = gal_tile_block_relative_to_other(tile, new); /* Do your processing.... in a loop (over many tiles). */ GAL_TILE_PARSE_OPERATE(tile, faketile, 1, 1, @{ YOUR_PROCESSING_EXPRESSIONS; @}); /* Clean up (outside the loop). */ faketile->array=NULL; faketile->dsize=NULL; gal_data_free(faketile); @end example @end deffn @node Tile grid, , Independent tiles, Tessellation library @subsubsection Tile grid One very useful application of tiles is to completely cover an input dataset with tiles. Such that you know every pixel/data-element of the input image is covered by only one tile. The constructs in this section allow easy definition of such a tile structure. They will create lists of tiles that are also usable by the general tools discussed in @ref{Independent tiles}. As discussed in @ref{Tessellation}, (mainly raw) astronomical images will mostly require two layers of tessellation, one for amplifier channels which all have the same size and another (smaller tile-size) tessellation over each channel. Hence, in this section we define a general structure to keep the main parameters of this two-layer tessellation and help in benefiting from it. @deftp {Type (C @code{struct})} gal_tile_two_layer_params This is the general structure to keep all the necessary parameters for a two-layer tessellation. @example struct gal_tile_two_layer_params @{ /* Inputs */ size_t *tilesize; /*******************************/ size_t *numchannels; /* These parameters have to be */ float remainderfrac; /* filled manually before */ uint8_t workoverch; /* calling the functions in */ uint8_t checktiles; /* this section. */ uint8_t oneelempertile; /*******************************/ /* Internal parameters. */ size_t ndim; size_t tottiles; size_t tottilesinch; size_t totchannels; size_t *channelsize; size_t *numtiles; size_t *numtilesinch; char *tilecheckname; size_t *permutation; size_t *firsttsize; /* Tile and channel arrays (which are also lists). */ gal_data_t *tiles; gal_data_t *channels; @}; @end example @end deftp @deftypefun {size_t *} gal_tile_full (gal_data_t @code{*input}, size_t @code{*regular}, float @code{remainderfrac}, gal_data_t @code{**out}, size_t @code{multiple}, size_t @code{**firsttsize}) Cover the full dataset with (mostly) identical tiles and return the number of tiles created along each dimension. The regular tile size (along each dimension) is determined from the @code{regular} array. If @code{input}'s size is not an exact multiple of @code{regular} for each dimension, then the tiles touching the edges in that dimension will have a different size to fully cover every element of the input (depending on @code{remainderfrac}). The output is an array with the same dimensions as @code{input} which contains the number of tiles along each dimension. See @ref{Tessellation} for a description of its application in Gnuastro's programs and @code{remainderfrac}, just note that this function defines only one layer of tiles. This is a low-level function (independent of the @code{gal_tile_two_layer_params} structure defined above). If you want a two-layer tessellation, directly call @code{gal_tile_full_two_layers} that is described below. The input arguments to this function are: @table @code @item input The main dataset (allocated block) which you want to create a tessellation over (only used for its sizes). So @code{input} may be a tile also. @item regular The the size of the regular tiles along each of the input's dimensions. So it must have the same number of elements as the dimensions of @code{input} (or @code{input->ndim}). @item remainderfrac The significant fraction of the remainder space to see if it should be split into two and put on both sides of a dimension or not. This is thus only relevant @code{input} length along a dimension isn't an exact multiple of the regular tile size along that dimension. See @ref{Tessellation} for a more thorough discussion. @item out Pointer to the array of data structures that will keep all the tiles (see @ref{Arrays of datasets}). If @code{*out==NULL}, then the necessary space to keep all the tiles will be allocated. If not, then all the tile information will be filled from the dataset that @code{*out} points to, see @code{multiple} for more. @item multiple When @code{*out==NULL} (and thus will be allocated by this function), allocate space for @code{multiple} times the number of tiles needed. This can be very useful when you have several more identically sized @code{inputs}, and you want all their tiles to be allocated (and thus indexed) together, even though they have different @code{block} datasets (that then link to one allocated space). See the definition of channels in @ref{Tessellation} and @code{gal_tile_full_two_layers} below. @item firsttsize The size of the first tile along every dimension. This is only different from the regular tile size when @code{regular} is not an exact multiple of @code{input}'s length along every dimension. This array is allocated internally by this function. @end table @end deftypefun @deftypefun void gal_tile_full_sanity_check (char @code{*filename}, char @code{*hdu}, gal_data_t @code{*input}, struct gal_tile_two_layer_params @code{*tl}) Make sure that the input parameters (in @code{tl}, short for two-layer) correspond to the input dataset. @code{filename} and @code{hdu} are only required for error messages. Also, allocate and fill the @code{tl->channelsize} array. @end deftypefun @deftypefun void gal_tile_full_two_layers (gal_data_t @code{*input}, struct gal_tile_two_layer_params @code{*tl}) Create the two layered tessellation in @code{tl}. The general set of steps you need to take to define the two-layered tessellation over an image can be seen in the example code below. @example gal_data_t *input; struct gal_tile_two_layer_params tl; char *filename="input.fits", *hdu="1"; /* Set all the inputs shown in the structure definition. */ ... /* Read the input dataset. */ input=gal_fits_img_read(filename, hdu, -1, 0, 0); /* Do a sanity check and preparations. */ gal_tile_full_sanity_check(filename, hdu, input, &tl); /* Build the two-layer tessellation*/ gal_tile_full_two_layers(input, &tl); /* `tl.tiles' and `tl.channels' are now a lists of tiles.*/ @end example @end deftypefun @deftypefun void gal_tile_full_permutation (struct gal_tile_two_layer_params @code{*tl}) Make a permutation to allow the conversion of tile location in memory to its location in the full input dataset and put it in @code{tl->permutation}. If a permutation has already been defined for the tessellation, this function will not do anything. If permutation won't be necessary (there is only one channel or one dimension), then this function will not do anything (@code{tl->permutation} must have been initialized to @code{NULL}). When there is only one channel OR one dimension, the tiles are allocated in memory in the same order that they represent the input data. However, to make channel-independent processing possible in a generic way, the tiles of each channel are allocated contiguously. So, when there is more than one channel AND more than one dimension, the index of the tile does not correspond to its position in the grid covering the input dataset. The example below may help clarify: assume you have a 6x6 tessellation with two channels in the horizontal and one in the vertical. On the left you can see how the tile IDs correspond to the input dataset. NOTE how `03' is on the second row, not on the first after `02'. On the right, you can see how the tiles are stored in memory (and shown if you simply write the array into a FITS file for example). @example Corresponding to input In memory ---------------------- -------------- 15 16 17 33 34 35 30 31 32 33 34 35 12 13 14 30 31 32 24 25 26 27 28 29 09 10 11 27 28 29 18 19 20 21 22 23 06 07 08 24 25 26 <-- 12 13 14 15 16 17 03 04 05 21 22 23 06 07 08 09 10 11 00 01 02 18 19 20 00 01 02 03 04 05 @end example As a result, if your values are stored in same order as the tiles, and you want them in over-all memory (for example to save as a FITS file), you need to permute the values: @example gal_permutation_apply(values, tl->permutation); @end example If you have values over-all and you want them in tile-order, you can apply the inverse permutation: @example gal_permutation_apply_inverse(values, tl->permutation); @end example Recall that this is the definition of permutation in this context: @example permute: IN_ALL[ i ] = IN_MEMORY[ perm[i] ] inverse: IN_ALL[ perm[i] ] = IN_MEMORY[ i ] @end example @end deftypefun @deftypefun void gal_tile_full_values_write (gal_data_t @code{*tilevalues}, struct gal_tile_two_layer_params @code{*tl}, int @code{withblank}, char @code{*filename}, gal_fits_list_key_t @code{*keys}, char @code{*program_string}) Write one value for each tile into a file. It is important to note that the values in @code{tilevalues} must be ordered in the same manner as the tiles, so @code{tilevalues->array[i]} is the value that should be given to @code{tl->tiles[i]}. The @code{tl->permutation} array must have been initialized before calling this function with @code{gal_tile_full_permutation}. If @code{withblank} is non-zero, then block structure of the tiles will be checked and all blank pixels in the block will be blank in the final output file also. @end deftypefun @deftypefun {gal_data_t *} gal_tile_full_values_smooth (gal_data_t @code{*tilevalues}, struct gal_tile_two_layer_params @code{*tl}, size_t @code{width}, size_t @code{numthreads}) Smooth the given values with a flat kernel of the given @code{width}. This cannot be done manually because if @code{tl->workoverch==0}, tiles in different channels must not be mixed/smoothed. Also the tiles are contiguous within the channel, not within the image, see the description under @code{gal_tile_full_permutation}. @end deftypefun @deftypefun size_t gal_tile_full_id_from_coord (struct gal_tile_two_layer_params @code{*tl}, size_t @code{*coord}) Return the ID of the tile that corresponds to the coordinates @code{coord}. Having this ID, you can use the @code{tl->tiles} array to get to the proper tile or read/write a value into an array that has one value per tile. @end deftypefun @deftypefun void gal_tile_full_free_contents (struct gal_tile_two_layer_params @code{*tl}) Free all the allocated arrays within @code{tl}. @end deftypefun @node Bounding box, Polygons, Tessellation library, Gnuastro library @subsection Bounding box (@file{box.h}) Functions related to reporting a the bounding box of certain inputs are declared in @file{gnuastro/box.h}. All coordinates in this header are in the FITS format (first axis is the horizontal and the second axis is vertical). @deftypefun void gal_box_bound_ellipse_extent (double @code{a}, double @code{b}, double @code{theta_deg}, double @code{*extent}) Return the maximum extent along each dimension of the given ellipse from the center of the ellipse. Therefore this is half the extent of the box in each dimension. @code{a} is the ellipse major axis, @code{b} is the minor axis, @code{theta_deg} is the position angle in degrees. The extent in each dimension is in floating point format and stored in @code{extent} which must already be allocated before this function. @end deftypefun @deftypefun void gal_box_bound_ellipse (double @code{a}, double @code{b}, double @code{theta_deg}, long @code{*width}) Any ellipse can be enclosed into a rectangular box. The purpose of this function is to give the height and width of that box assuming the center of the ellipse is in the box center. @code{a} is the ellipse major axis, @code{b} is the minor axis, @code{theta_deg} is the position angle in degrees. The @code{width} array will contain the output size in long integer type. @code{width[0]}, and @code{width[1]} are the number of pixels along the first and second FITS axis. Since the ellipse center is assumed to be in the center of the box, all the values in @code{width} will be an odd integer. @end deftypefun @deftypefun void gal_box_border_from_center (double @code{center}, size_t @code{ndim}, long @code{*width}, long @code{*fpixel}, long @code{*lpixel}) Given the center coordinates in @code{center} and the @code{width} (along each dimension) of a box, return the coordinates of the first (@code{fpixel}) and last (@code{lpixel}) pixels. All arrays must have @code{ndim} elements (one for each dimension). @end deftypefun @deftypefun int gal_box_overlap (long @code{*naxes}, long @code{*fpixel_i}, long @code{*lpixel_i}, long @code{*fpixel_o}, long @code{*lpixel_o}, size_t @code{ndim}) An @code{ndim}-dimensional dataset of size @code{naxes} (along each dimension, in FITS order) and a box with first and last (inclusive) coordinate of @code{fpixel_i} and @code{lpixel_i} is given. This box doesn't necessarily have to lie within the dataset, it can be outside of it, or only patially overlap. This function will change the values of @code{fpixel_i} and @code{lpixel_i} to exactly cover the overlap in the input dataset's coordinates. This function will return 1 if there is an overlap and 0 if there isn't. When there is an overlap, the coordinates of the first and last pixels of the overlap will be put in @code{fpixel_o} and @code{lpixel_o}. @end deftypefun @node Polygons, Qsort functions, Bounding box, Gnuastro library @subsection Polygons (@file{polygon.h}) Polygons are commonly necessary in image processing. In Gnuastro, they are used in Crop (see @ref{Crop}) for cutting out non-rectangular regions of a image. Warp (see @ref{Warp}) uses them to warp the images into a new pixel grid. The polygon related Gnuastro library macros and functions are introduced here. In all the functions here the vertices (and points) are defined as an array. So a polygon with 4 vertices will be identified with an array of 8 elements with the first two elements keeping the 2D coordinates of the first vertice and so on. @deffn Macro GAL_POLYGON_MAX_CORNERS The largest number of vertices a polygon can have in this library. @end deffn @deffn Macro GAL_POLYGON_ROUND_ERR @cindex Round-off error We have to consider floating point round-off errors when dealing with polygons. For example we will take @code{A} as the maximum of @code{A} and @code{B} when @code{A>B-GAL_POLYGON_ROUND_ERR}. @end deffn @deftypefun void gal_polygon_ordered_corners (double @code{*in}, size_t @code{n}, size_t @code{*ordinds}) We have a simple polygon (that can result from projection, so its edges don't collide or it doesn't have holes) and we want to order its corners in an anticlockwise fashion. This is necessary for clipping it and finding its area later. The input vertices can have practically any order. The input (@code{in}) is an array containing the coordinates (two values) of each vertice. @code{n} is the number of corners. So @code{in} should have @code{2*n} elements. The output (@code{ordinds}) is an array with @code{n} elements specifying the indexs in order. This array must have been allocated before calling this function. The indexes are output for more generic usage, for example in a homographic transform (necessary in warping an image, see @ref{Warping basics}), the necessary order of vertices is the same for all the pixels. In other words, only the positions of the vertices change, not the way they need to be ordered. Therefore, this function would only be necessary once. As a summary, the input is unchanged, only @code{n} values will be put in the @code{ordinds} array. Such that calling the input coordinates in the following fashion will give an anti-clockwise order when there are 4 vertices: @example 1st vertice: in[ordinds[0]*2], in[ordinds[0]*2+1] 2nd vertice: in[ordinds[1]*2], in[ordinds[1]*2+1] 3rd vertice: in[ordinds[2]*2], in[ordinds[2]*2+1] 4th vertice: in[ordinds[3]*2], in[ordinds[3]*2+1] @end example @cindex Convex Hull @noindent The implementation of this is very similar to the Graham scan in finding the Convex Hull. However, in projection we will never have a concave polygon (the left condition below, where this algorithm will get to E before D), we will always have a convex polygon (right case) or E won't exist! @example Concave Polygon Convex Polygon D --------C D------------- C \ | E / | \E | \ | / | \ | A--------B A ----------B @end example This is because we are always going to be calculating the area of the overlap between a quadrilateral and the pixel grid or the quadrilateral its self. The @code{GAL_POLYGON_MAX_CORNERS} macro is defined so there will be no need to allocate these temporary arrays separately. Since we are dealing with pixels, the polygon can't really have too many vertices. @end deftypefun @deftypefun double gal_polygon_area (double @code{*v}, size_t @code{n}) Find the area of a polygon with vertices defined in @code{v}. @code{v} points to an array of doubles which keep the positions of the vertices such that @code{v[0]} and @code{v[1]} are the positions of the first vertice to be considered. @end deftypefun @deftypefun int gal_polygon_pin (double @code{*v}, double @code{*p}, size_t @code{n}) Return @code{1} if the point @code{p} is within the polygon whose vertices are defined by @code{v} and @code{0} otherwise. Note that the vertices of the polygon have to be sorted in an anti-clock-wise manner. @end deftypefun @deftypefun int gal_polygon_ppropin (double @code{*v}, double @code{*p}, size_t @code{n}) Similar to @code{gal_polygon_pin}, except that if the point @code{p} is on one of the edges of a polygon, this will return @code{0}. @end deftypefun @deftypefun void gal_polygon_clip (double @code{*s}, size_t @code{n}, double @code{*c}, size_t @code{m}, double @code{*o}, size_t @code{*numcrn}) Clip (find the overlap of) two polygons. This function uses the @url{https://en.wikipedia.org/wiki/Sutherland%E2%80%93Hodgman_algorithm, Sutherland-Hodgman} polygon clipping algorithm. Note that the vertices of both polygons have to be sorted in an anti-clock-wise manner. @end deftypefun @node Qsort functions, Permutations, Polygons, Gnuastro library @subsection Qsort functions (@file{qsort.h}) The C programming language comes with the @code{qsort} (Quick sort) function. @code{qsort} is a generic function which allows you to sort any kind of data structure (not just a single number). To define greater and smaller (for sorting), @code{qsort} needs another function, even for simple numerical types. To facilitate numerical sorting for Gnuastro's programs/libraries, Gnuastro defines a function for each type's increasing and decreasing function. You can pass these functions to @code{qsort} when your array has the respective type (see @ref{Numeric data types}). @deffn {Global variable} {gal_qsort_index_arr} Pointer to a floating point array (@code{float *}) to use as a reference in @code{gal_qsort_index_float_decreasing}, see the explanation there for more. @end deffn @deftypefun int gal_qsort_index_float_decreasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort a @code{size_t} array based on decreasing values in the @code{gal_qsort_index_arr} single precision floating point array. The floating point array will not be changed, it is only read. For example, if we have the following source code: @example #include #include /* qsort is defined in stdlib.h. */ #include int main (void) @{ size_t s[4]=@{0, 1, 2, 3@}; float f[4]=@{1.3,0.2,1.8,0.1@}; gal_qsort_index_arr=f; qsort(s, 4, sizeof(size_t), gal_qsort_index_float_decreasing); printf("%zu, %zu, %zu, %zu\n", s[0], s[1], s[2], s[3]); return EXIT_SUCCESS; @} @end example @noindent The output will be: @code{2, 0, 1, 3}. @end deftypefun @deftypefun int gal_qsort_TYPE_increasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort an @code{TYPE} array in increasing order (first element will be the smallest). Please replace @code{TYPE} (in the function name) with one of the @ref{Numeric data types}, for example @code{gal_qsort_int32_increasing}, or @code{gal_qsort_float64_increasing}. @end deftypefun @deftypefun int gal_qsort_TYPE_decreasing (const void @code{*a}, const void @code{*b}) When passed to @code{qsort}, this function will sort an @code{TYPE} array in decreasing order (first element will be the largest). Please replace @code{TYPE} (in the function name) with one of the @ref{Numeric data types}, for example @code{gal_qsort_int32_decreasing}, or @code{gal_qsort_float64_decreasing}. @end deftypefun @node Permutations, Matching, Qsort functions, Gnuastro library @subsection Permutations (@file{permutation.h}) @cindex permutation Permutation is the technical name for re-ordering of values. The need for permutations occurs a lot during (mainly low-level) processing. To do permutation, you must provide two inputs: an array of values (that you want to re-order in place) and a permutation array which contains the new index of each element (let's call it @code{perm}). The diagram below shows the input array before and after the re-ordering. @example permute: AFTER[ i ] = BEFORE[ perm[i] ] i = 0 .. N-1 inverse: AFTER[ perm[i] ] = BEFORE[ i ] i = 0 .. N-1 @end example @cindex GNU Scientific Library The functions here are a re-implementation of the GNU Scientific Library's @code{gsl_permute} function. The reason we didn't use that function was that it uses system-specific types (like @code{long} and @code{int}) which can have different widths on different systems, hence are not easily convertible to Gnuastro's fixed width types (see @ref{Numeric data types}). There is also a separate function for each type, heavily using macros to allow a @code{base} function to work on all the types. Thus it is hard to read/understand. Hence, Gnuastro contains a re-write of their steps in a new type-agnostic method which is a single function that can work on any type. As described in GSL's source code and manual, this implementation comes from Donald Knuth's @emph{Art of computer programming} book, in the "Sorting and Searching" chapter of Volume 3 (3rd ed). Exercise 10 of Section 5.2 defines the problem and in the answers, Knuth describes the solution. So if you are interested, please have a look there for more. We are in contact with the GSL developers and in the future@footnote{Gnuastro's @url{http://savannah.gnu.org/task/?14497, Task 14497}. If this task is still ``postponed'' when you are reading this and you are interested to help, your help would be very welcome. Both Gnuastro and GSL developers are very busy, hence both would appreciate your help.} we will submit these implementations to GSL. If they are finally incorporated there, we will delete this section in future versions. @deftypefun void gal_permutation_check (size_t @code{*permutation}, size_t @code{size}) Print how @code{permutation} will re-order an array that has @code{size} elements for each element in one one line. @end deftypefun @deftypefun void gal_permutation_apply (gal_data_t @code{*input}, size_t @code{*permutation}) Apply @code{permutation} on the @code{input} dataset (can have any type), see above for the definition of permutation. @end deftypefun @deftypefun void gal_permutation_apply_inverse (gal_data_t @code{*input}, size_t @code{*permutation}) Apply the inverse of @code{permutation} on the @code{input} dataset (can have any type), see above for the definition of permutation. @end deftypefun @node Matching, Statistical operations, Permutations, Gnuastro library @subsection Matching (@file{match.h}) Matching is often necessary when the measurements have been done using different instruments, different software or different configurations of the same software. The functions in this part of Gnuastro's library will be growing to allow matching of images and finding a match between different catalogs (register them). Currently it only provides the The high-level measurements are stored in tables with positions (commonly in RA and Dec with units of degrees). @deftypefun {gal_data_t *} gal_match_coordinates (gal_data_t @code{*coord1}, gal_data_t @code{*coord2}, double @code{*aperture}, int @code{sorted_by_first}, int @code{inplace}, size_t @code{minmapsize}, size_t @code{*nummatched}) Return the permutations that when applied, the first @code{nummatched} rows of both inputs match with each other (are the nearest within the given aperture). The two inputs (@code{coord1} and @code{coord2}) must be @ref{List of gal_data_t}. Each @code{gal_data_t} node in the list should be a single dimensional dataset (column in a table). The dimensions of the coordinates is determined by the number of @code{gal_data_t} nodes in the two input lists (which must be equal). Note that the number of rows (or the number of elements in each @code{gal_data_t}) in the columns of @code{coord1} and @code{coord2} can be different. The matching aperture is defined by the @code{aperture} array. If several points of one catalog lie within this aperture of a point in the other, the nearest is defined as the match. In a 2D situation (where the input lists have two nodes), for the most generic case, it must have three elements: the major axis length, axis ratio and position angle (see @ref{Defining an ellipse}). If @code{aperture[1]==1}, the aperture will be a circle of radius @code{aperture[0]} and the third value won't be used. When the aperture is an ellipse, distances between the points are also calculated in the respective elliptical distances (@mymath{r_{el}} in @ref{Defining an ellipse}). To speed up the search, this function will sort the input coordinates by their first column (first axis). If @emph{both} are already sorted by their first column, you can avoid the sorting step by giving a non-zero value to @code{sorted_by_first}. When sorting is necessary and @code{inplace} is non-zero, the actual input columns will be sorted. Otherwise, an internal copy of the inputs will be made, used (sorted) and later freed before returning. Therefore, when @code{inplace==0}, inputs will remain untouched, but this function will take more time and memory. If internal allocation is necessary and the space is larger than @code{minmapsize}, the space will be not allocated in the RAM, but in a file, see description of @option{--minmapsize} in @ref{Processing options}. The number of matches will be put in the space pointed by @code{nummatched}. If there wasn't any match, this function will return @code{NULL}. If match(s) were found, a list with three @code{gal_data_t} nodes will be returned. The top two nodes in the list are the permutations that must be applied to the first and second inputs respectively. After applying the permutations, the top @code{nummatched} elements will match with each other. The third node is the distances between the respective match. Note that the three nodes of the list are all one-dimensional (a column) and can have different lengths. @cartouche @noindent @strong{Output permutations ignore internal sorting}: the output permutations will correspond to the initial inputs. Therefore, even when @code{inplace!=0} (and this function re-arranges the inputs), the output permutation will correspond to original (possibly non-sorted) inputs. The reason for this is that you rarely want the actual positional columns after the match. Usually, you also have other columns (measurements, for example magnitudes) for higher-level processing after the match (that correspond to the input order before sorting). Once you have the permutations, they can be applied to those other columns (see @ref{Permutations}) and the higher-level processing can continue. @end cartouche When you read the coordinates from a table using @code{gal_table_read} (see @ref{Table input output}), and only ask for the coordinate columns, the inputs to this function are the returned @code{gal_data_t *} from two different tables. @end deftypefun @node Statistical operations, Binary datasets, Matching, Gnuastro library @subsection Statistical operations (@file{statistics.h}) After reading a dataset into memory from a file or fully simulating it with another process, the most common processes that will be done on it are statistical operations to let you quantify different aspects of the data. the functions in this section describe Gnuastro's current set of tools for this job. All these functions can work on any numeric data type natively (see @ref{Numeric data types}) and can also work on tiles over a dataset. Hence the inputs and outputs are in Gnuastro's @ref{Generic data container}. @deffn Macro GAL_STATISTICS_SIG_CLIP_MAX_CONVERGE The maximum number of clips, when @mymath{\sigma}-clipping should be done by convergence. If the clipping does not converge before making this many clips, all sigma-clipping outputs will be NaN. @end deffn @deffn Macro GAL_STATISTICS_MODE_GOOD_SYM The minimum acceptable symmetricity of the mode calculation. If the symmetricity of the derived mode is less than this value, all the returned values by @code{gal_statistics_mode} will have a value of NaN. @end deffn @deffn Macro GAL_STATISTICS_SORTED_NOT @deffnx Macro GAL_STATISTICS_SORTED_INCREASING @deffnx Macro GAL_STATISTICS_SORTED_DECREASING Macros used to identify if the dataset is sorted and increasing, sorted and decreasing or not sorted. @end deffn @deffn Macro GAL_STATISTICS_BINS_INVALID @deffnx Macro GAL_STATISTICS_BINS_REGULAR @deffnx Macro GAL_STATISTICS_BINS_IRREGULAR Macros used to identify if the regularity of the bins when defining bins. @end deffn @cindex Number @deftypefun {gal_data_t *} gal_statistics_number (gal_data_t @code{*input}) Return a single-element @code{uint64} dataset containing the number of non-blank elements in @code{input}. @end deftypefun @cindex Minimum @deftypefun {gal_data_t *} gal_statistics_minimum (gal_data_t @code{*input}) Return a single-element dataset containing the minimum non-blank value in @code{input}. The numerical datatype of the output is the same as @code{input}. @end deftypefun @cindex Maximum @deftypefun {gal_data_t *} gal_statistics_maximum (gal_data_t @code{*input}) Return a single-element dataset containing the maximum non-blank value in @code{input}. The numerical datatype of the output is the same as @code{input}. @end deftypefun @cindex Sum @deftypefun {gal_data_t *} gal_statistics_sum (gal_data_t @code{*input}) Return a single-element (@code{double} or @code{float64}) dataset containing the sum of the non-blank values in @code{input}. @end deftypefun @cindex Mean @cindex Average @deftypefun {gal_data_t *} gal_statistics_mean (gal_data_t @code{*input}) Return a single-element (@code{double} or @code{float64}) dataset containing the mean of the non-blank values in @code{input}. @end deftypefun @cindex Standard deviation @deftypefun {gal_data_t *} gal_statistics_std (gal_data_t @code{*input}) Return a single-element (@code{double} or @code{float64}) dataset containing the standard deviation of the non-blank values in @code{input}. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_mean_std (gal_data_t @code{*input}) Return a two-element (@code{double} or @code{float64}) dataset containing the mean and standard deviation of the non-blank values in @code{input}. The first element of the returned dataset is the mean and the second is the standard deviation. This function will calculate both values in one pass over the dataset. Hence when both the mean and standard deviation of a dataset are necessary, this function is much more efficient than calling @code{gal_statistics_mean} and @code{gal_statistics_std} separately. @end deftypefun @cindex Median @deftypefun {gal_data_t *} gal_statistics_median (gal_data_t @code{*input}, int @code{inplace}) Return a single-element dataset containing the median of the non-blank values in @code{input}. The numerical datatype of the output is the same as @code{input}. Calculating the median involves sorting the dataset and removing blank values, for better performance (and less memory usage), you can give a non-zero value to the @code{inplace} argument. In this case, the sorting and removal of blank elements will be done directly on the input dataset. However, after this function the original dataset may have changed (if it wasn't sorted or had blank values). @end deftypefun @cindex Quantile @deftypefun size_t gal_statistics_quantile_index (size_t @code{size}, double @code{quantile}) Return the index of the element that has a quantile of @code{quantile} assuming the dataset has @code{size} elements. @end deftypefun @deftypefun size_t gal_statistics_quantile (gal_data_t @code{*input}, double @code{quantile}, int @code{inplace}) Return a single-element dataset containing the value with in a quantile @code{quantile} of the non-blank values in @code{input}. The numerical datatype of the output is the same as @code{input}. See @code{gal_statistics_median} for a description of @code{inplace}. @end deftypefun @deftypefun size_t gal_statistics_quantile_function_index (gal_data_t @code{*input}, gal_data_t @code{*value}, int @code{inplace}) Return the index of the quantile function (inverse quantile) of @code{input} at @code{value}. In other words, this function will return the index of the nearest element (of a sorted and non-blank) @code{input} to @code{value}. See @code{gal_statistics_median} for a description of @code{inplace}. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_quantile_function (gal_data_t @code{*input}, gal_data_t @code{*value}, int @code{inplace}) Return a single-element (@code{double} or @code{float64}) dataset containing the quantile function of the non-blank values in @code{input} at @code{value}. In other words, this function will return the quantile of @code{value} in @code{input}. See @code{gal_statistics_median} for a description of @code{inplace}. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_mode (gal_data_t @code{*input}, float @code{mirrordist}, int @code{inplace}) Return a four-element (@code{double} or @code{float64}) dataset that contains the mode of the @code{input} distribution. This function implements the non-parametric algorithm to find the mode that is described in Appendix C of @url{https://arxiv.org/abs/1505.01664, Akhlaghi and Ichikawa [2015]}. In short it compares the actual distribution and its ``mirror distribution'' to find the mode. In order to be efficient, you can determine how far the comparison goes away from the mirror through the @code{mirrordist} parameter (think of it as a multiple of sigma/error). See @code{gal_statistics_median} for a description of @code{inplace}. The output array has the following elements (in the given order, note that counting in C starts from 0). @example array[0]: mode array[1]: mode quantile. array[2]: symmetricity. array[3]: value at the end of symmetricity. @end example @end deftypefun @deftypefun {gal_data_t *} gal_statistics_mode_mirror_plots (gal_data_t @code{*input}, gal_data_t @code{*value}, size_t @code{numbins}, int @code{inplace}, double @code{*mirror_val}) Make a mirrored histogram and cumulative frequency plot (with @code{numbins}) with the mirror distribution of the @code{input} with a value at @code{value}. The output is a list of data structures (see @ref{List of gal_data_t}): the first is the bins with one bin at the mirror point, the second is the histogram with a maximum of one and the third is the cumulative frequency plot (with a maximum of one). @end deftypefun @deftypefun int gal_statistics_is_sorted (gal_data_t @code{*input}) Return the respective sort macro (see above) for the @code{input} dataset. @end deftypefun @deftypefun void gal_statistics_sort_increasing (gal_data_t @code{*input}) Sort the input dataset (in place) in an increasing order. @end deftypefun @deftypefun void gal_statistics_sort_decreasing (gal_data_t @code{*input}) Sort the input dataset (in place) in a decreasing order. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_no_blank_sorted (gal_data_t @code{*input}, int @code{inplace}) Remove all the blanks and sort the input dataset. If @code{inplace} is non-zero this will happen on the input dataset (and the output will be the same as the input). However, if @code{inplace} is zero, this function will allocate a new copy of the dataset that is sorted and has no blank values. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_regular_bins (gal_data_t @code{*input}, gal_data_t @code{*inrange}, size_t @code{numbins}, double @code{onebinstart}) Generate an array of regularly spaced elements as a 1D array (column) of type @code{double} (i.e., @code{float64}, it has to be double to account for small differences on the bin edges). The input arguments are described below @table @code @item input The dataset you want to apply the bins to. This is only necessary if the range argument is not complete, see below. If @code{inrange} has all the necessary information, you can pass a @code{NULL} pointer for this. @item inrange This dataset keeps the desired range along each dimension of the input data structure, it has to be in @code{float} (i.e., @code{float32}) type. @itemize @item If you want the full range of the dataset (in any dimensions, then just set @code{inrange} to @code{NULL} and the range will be specified from the minimum and maximum value of the dataset (@code{input} cannot be @code{NULL} in this case). @item If there is one element for each dimension in range, then it is viewed as a quantile (Q), and the range will be: `Q to 1-Q'. @item If there are two elements for each dimension in range, then they are assumed to be your desired minimum and maximum values. When either of the two are NaN, the minimum and maximum will be calculated for it. @end itemize @item numbins The number of bins: must be larger than 0. @item onebinstart A desired value for onebinstart. Note that with this option, the bins won't start and end exactly on the given range values, it will be slightly shifted to accommodate this request. @end table @end deftypefun @deftypefun {gal_data_t *} gal_statistics_histogram (gal_data_t @code{*input}, gal_data_t @code{*bins}, int @code{normalize}, int @code{maxone}) Make a histogram of all the elements in the given dataset with bin values that are defined in the @code{inbins} structure (see @code{gal_statistics_regular_bins}). @code{inbins} is not mandatory, if you pass a @code{NULL} pointer, the bins structure will be built within this function based on the @code{numbins} input. As a result, when you have already defined the bins, @code{numbins} is not used. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_cfp (gal_data_t @code{*input}, gal_data_t @code{*bins}, int @code{normalize}) Make a cumulative frequency plot (CFP) of all the elements in @code{input} with bin values that are defined in the @code{bins} structure (see @code{gal_statistics_regular_bins}). The CFP is built from the histogram: in each bin, the value is the sum of all previous bins in the histogram. Thus, if you have already calculated the histogram before calling this function, you can pass it onto this function as the data structure in @code{bins->next} (see @code{List of gal_data_t}). If @code{bin->next!=NULL}, then it is assumed to be the histogram. If it is @code{NULL}, then the histogram will be calculated internally and freed after the job is finished. When a histogram is given and it is normalized, the CFP will also be normalized (even if the normalized flag is not set here): note that a normalized CFP's maximum value is 1. @end deftypefun @deftypefun {gal_data_t *} gal_statistics_sigma_clip (gal_data_t @code{*input}, float @code{multip}, float @code{param}, int @code{inplace}, int @code{quiet}) Apply @mymath{\sigma}-clipping on a given dataset and return a dataset that contains the results. For a description of @mymath{\sigma}-clipping see @ref{Sigma clipping}. @code{multip} is the multiple of the standard deviation (@mymath{\sigma} that is used to define outliers in each round of clipping). The role of @code{param} is determined based on its value. If @code{param} is larger than @code{1} (one), it must be an integer and will be interpretted as the number clips to do. If it is less than @code{1} (one), it is interpretted as the tolerance level to stop the iteration. The output dataset has the following elements with a @code{GAL_TYPE_FLOAT32} type: @example array[0]: Number of points used. array[1]: Median. array[2]: Mean. array[3]: Standard deviation. @end example @end deftypefun @node Binary datasets, Convolution functions, Statistical operations, Gnuastro library @subsection Binary datasets (@file{binary.h}) @cindex Thresholding @cindex Binary datasets @cindex Dataset: binary Binary datasets only have two (usable) values: 0 (also known as background) or 1 (also known as foreground). They are created after some binary classification is applied to the dataset. The most common is thresholding: for example in an image, pixels with a value above the threshold are given a value of 1 and those with a value less than the threshold are assigned a value of 0. @cindex Connectivity @cindex Immediate neighbors @cindex Neighbors, immediate Since there is only two values, in the processing of binary images, you are usually concerned with the positioning of an element and its vicinity (neighbors). When a dataset has more than one dimension, multiple classes of immediate neighbors (that are touching the element) can be defined for each data-element. To separate these different classes of immediate neighbors, we define @emph{connectivity}. The classification is done by the distance from element center to the neighbor's center. The nearest immediate neighbors have a connectivity of 1, the second nearest class of neighbors have a connectivity of 2 and so on. In total, the largest possible connectivity for data with @code{ndim} dimensions is @code{ndim}. For example in a 2D dataset, 4-connected neighbors (that share an edge and have a distance of 1 pixel) have a connectivity of 1. The other 4 neighbors that only share a vertice (with a distance of @mymath{\sqrt{2}} pixels) have a connectivity of 2. Conventionally, the class of connectivity-2 neighbors also includes the connectivity 1 neighbors, so for example we call them 8-connected neighbors in 2D datasets. Ideally, one bit is sufficient for each element of a binary dataset. However, CPUs are not designed to work on individual bits, the smallest unit of memory addresses is a byte (containing 8 bits on modern CPUs). Therefore, in Gnuastro, the type used for binary dataset is @code{uint8_t} (see @ref{Numeric data types}). Although it does take 8-times more memory, this choice offers much better performance and the some extra (useful) features. The advantage of using a full byte for each element of a binary dataset is that you can also have other values (that will be ignored in the processing). One such common ``other'' value in real datasets is a blank value (to mark regions that should not be processed because there is no data). The constant @code{GAL_BLANK_UINT8} value must be used in these cases (see @ref{Library blank values}). Another is some temporary value(s) that can be given to a processed pixel to avoid having another copy of the dataset as in @code{GAL_BINARY_TMP_VALUE} that is described below. @deffn Macro GAL_BINARY_TMP_VALUE The functions described below work on a @code{uint8_t} type dataset with values of 1 or 0 (no other pixel will be touched). However, in some cases, it is necessary to put temporary values in each element during the processing of the functions. This temporary value has a special meaning for the operation and will be operated on. So if your input datasets have values other than 0 and 1 that you don't want these functions to work on, be sure they are not equal to this macro's value. Note that this value is also different from @code{GAL_BLANK_UINT8}, so your input datasets may also contain blank elements. @end deffn @deftypefun {gal_data_t *} gal_binary_erode (gal_data_t @code{*input}, size_t @code{num}, int @code{connectivity}, int @code{inplace}) Do @code{num} erosions on the @code{connectivity}-connected neighbors of @code{input} (see above for the definition of connectivity). If @code{inplace} is non-zero @emph{and} the input's type is @code{GAL_TYPE_UINT8}, then the erosion will be done within the input dataset and the returned pointer will be @code{input}. Otherwise, @code{input} is copied (and converted if necessary) to @code{GAL_TYPE_UINT8} and erosion will be done on this new dataset which will also be returned. This function will only work on the elements with a value of 1 or 0. It will leave all the rest unchanged. @cindex Erosion @cindex Mathematical morphology Erosion (inverse of dilation) is an operation in mathematical morphology where each foreground pixel that is touching a background pixel is flipped (changed to background). The @code{connectivity} value determines the definition of ``touching''. Erosion will thus decrease the area of the foreground regions by one layer of pixels. @end deftypefun @deftypefun {gal_data_t *} gal_binary_dilate (gal_data_t @code{*input}, size_t @code{num}, int @code{connectivity}, int @code{inplace}) Do @code{num} dilations on the @code{connectivity}-connected neighbors of @code{input} (see above for the definition of connectivity). For more on @code{inplace} and the output, see @code{gal_binary_erode}. @cindex Dilation Dilation (inverse of erosion) is an operation in mathematical morphology where each background pixel that is touching a foreground pixel is flipped (changed to foreground). The @code{connectivity} value determines the definition of ``touching''. Dilation will thus increase the area of the foreground regions by one layer of pixels. @end deftypefun @deftypefun {gal_data_t *} gal_binary_open (gal_data_t @code{*input}, size_t @code{num}, int @code{connectivity}, int @code{inplace}) Do @code{num} openings on the @code{connectivity}-connected neighbors of @code{input} (see above for the definition of connectivity). For more on @code{inplace} and the output, see @code{gal_binary_erode}. @cindex Opening (Mathematical morphology) Opening is an operation in mathematical morphology which is defined as erosion followed by dilation (see above for the definitions of erosion and dilation). Opening will thus remove the outer structure of the foreground. In this implementation, @code{num} erosions are going to be applied on the dataset, then @code{num} dilations. @end deftypefun @deftypefun size_t gal_binary_connected_components (gal_data_t @code{*binary}, gal_data_t @code{**out}, int @code{connectivity}) @cindex Connected components @cindex Breadth first search Return the number of connected components in @code{binary} through the breadth first search algorithm (finding all pixels belonging to one component before going on to the next). Connection between two pixels is defined based on the value to @code{connectivity}. @code{out} is a dataset with the same size as @code{binary} with @code{GAL_TYPE_INT32} type. Every pixel in @code{out} will have the label of the connected component it belongs to. The labeling of connected components starts from 1, so a label of zero is given to the input's background pixels. When @code{*out!=NULL} (its space is already allocated), it will be cleared (to zero) at the start of this function. Otherwise, when @code{*out==NULL}, the necessary dataset to keep the output will be allocated by this function. @code{binary} must have a type of @code{GAL_TYPE_UINT8}, otherwise this function will abort with an error. Other than blank pixels (with a value of @code{GAL_BLANK_UINT8} defined in @ref{Library blank values}), all other non-zero pixels in @code{binary} will be considered as foreground (and will be labeled). Blank pixels in the input will also be blank in the output. @end deftypefun @deftypefun {gal_data_t *} gal_binary_connected_adjacency_matrix (gal_data_t @code{*adjacency}, size_t @code{*numconnected}) @cindex Adjacency matrix @cindex Matrix, adjacency Find the number of connected labels and new labels based on an adjacency matrix, which must be a square binary array (type @code{GAL_TYPE_UINT8}). The returned dataset is a list of new labels for each old label. In other words, this function will find the objects that are connected (possibly through a third object) and in the output array, the respective elements for all input labels is going to have the same value. The total number of connected labels is put into the space that @code{numconnected} points to. An adjacency matrix defines connection between two labels. For example, let's assume we have 5 labels and we know that labels 1 and 5 are connected to label 3, but are not connected with each other. Also, labels 2 and 4 are not touching any other label. So in total we have 3 final labels: one combined object (merged from labels 1, 3, and 5) and the initial labels 2 and 4. The input adjacency matrix would look like this (note the extra row and column for a label 0 which is ignored): @example INPUT OUTPUT ===== ====== in_lab 1 2 3 4 5 | | numconnected = 3 0 0 0 0 0 0 | in_lab 1 --> 0 0 0 1 0 0 | in_lab 2 --> 0 0 0 0 0 0 | Returned: new labels for the in_lab 3 --> 0 1 0 0 0 1 | 5 initial objects in_lab 4 --> 0 0 0 0 0 0 | | 0 | 1 | 2 | 1 | 3 | 1 | in_lab 5 --> 0 0 0 1 0 0 | @end example Although the adjacency matrix as used here is symmetric, currently this function assumes that it is filled on both sides of the diagonal. @end deftypefun @deftypefun void gal_binary_fill_holes (gal_data_t @code{*input}, int @code{connectivity}) Fill all the holes (0 valued pixels surrounded by 1 valued pixels) within a region of the binary @code{input} dataset. The connectivity of the holes can be set with @code{connectivity}. This function currently only works on a 2D dataset. @end deftypefun @node Convolution functions, Interpolation, Binary datasets, Gnuastro library @subsection Convolution functions (@file{convolve.h}) Convolution is a very common operation during data analysis and is thoroughly described as part of Gnuastro's @ref{Convolve} program which is fully devoted to this job. Because of the complete introduction that was presented there, we will directly skip onto the currently available convolution functions in Gnuastro's library. As of this version, only spatial domain convolution is available in Gnuastro's libraries. We haven't had the time to liberate the frequency domain function convolution and de-convolution functions that are available in the Convolve program@footnote{Hence any help would be greatly appreciated.}. @deftypefun {gal_data_t *} gal_convolve_spatial (gal_data_t @code{*tiles}, gal_data_t @code{*kernel}, size_t @code{numthreads}, int @code{edgecorrection}, int @code{convoverch}) Convolve each node of the list of @code{tiles} (see @ref{List of gal_data_t} and @ref{Tessellation library}) with @code{kernel} using @code{numthreads}. When @code{edgecorrection} is non-zero, it will correct for the edge dimming effects as discussed in @ref{Edges in the spatial domain}. To create a tessellation that fully covers an input image, you may use @code{gal_tile_full}, or @code{gal_tile_full_two_layers} to also define channels over your input dataset. These functions are discussed in @ref{Tile grid}. You may then pass the list of tiles to this function. This is the recommended way to call this function because spatial domain convolution is slow and breaking the job into many small tiles and working on simultaneously on several threads can greatly speed up the processing. If the tiles are defined within a channel (a larger tile), by default convolution will be done within the channel, so pixels on the edge of a channel will not be affected by their neighbors that are in another channel. See @ref{Tessellation} for the necessity of channels in astronomical data analysis. This behavior may be disabled when @code{convoverch} is non-zero. In this case, it will ignore channel borders (if they exist) and mix all pixels that cover the kernel within the dataset. @end deftypefun @deftypefun void gal_convolve_spatial_correct_ch_edge (gal_data_t @code{*tiles}, gal_data_t @code{*kernel}, size_t @code{numthreads}, int @code{edgecorrection}, gal_data_t @code{*tocorrect}) Correct the edges of channels in an already convolved image when it was initially convolved with @code{gal_convolve_spatial} and @code{convoverch==0}. In that case, strong boundaries might exist on the channel edges. So if you later need to remove those boundaries at later steps of your processing, you can call this function. It will only do convolution on the tiles that are near the edge and were effected by the channel borders. Other pixels in the image will not be touched. Hence, it is much faster. @end deftypefun @node Interpolation, Git wrappers, Convolution functions, Gnuastro library @subsection Interpolation (@file{interpolate.h}) During data analysis, it often happens that parts of the data cannot be given a value. For example your image was saturated due to a very bright start and you have to mask that star's footprint. One other common situation in Gnuastro is when we do processing on tiles (for example to estimate the Sky value and its Standard deviation, see @ref{Sky value}). Some tiles must not be used for the estimation of the Sky value, for example because they cover a large galaxy. So we need to fill them in with blank values. But ultimately, we need a Sky value for every pixel. This job (assigning a value to blank element(s) based on their nearby neighbors with a value) is known as interpolation. There are many ways to do interpolation, but (mainly due to lack of time), currently Gnuastro only contains the (median of) nearest-neighbor method. The power of this method of interpolation is its non-parametric nature. The produced values are also always within the range of the known values and strong outliers do not get created. We will hopefully implement other methods too (wrappers around the GNU Scientific Library's very complete set of functions), but currently the developers are too busy. So if you do have the chance to help your contribution would be very welcome and appreciated. @deftypefun {gal_data_t *} gal_interpolate_close_neighbors (gal_data_t @code{*input}, struct gal_tile_two_layer_params @code{*tl}, size_t @code{numneighbors}, size_t @code{numthreads}, int @code{onlyblank}, int @code{aslinkedlist}) Interpolate the values in the image using the median value of their @code{numneighbors} closest neighbors. If @code{onlyblank} is non-zero, then only blank elements will be interpolated and pixels that already have a value will be left untouched. This function is multi-threaded and will run on @code{numthreads} threads (see @code{gal_threads_number} in @ref{Multithreaded programming}). @code{tl} is Gnuastro's two later tessellation structure used to define tiles over an image and is fully described in @ref{Tile grid}. When @code{tl!=NULL}, then it is assumed that the @code{input->array} contains one value per tile and interpolation will respect certain tessellation properties, for example to not interpolate over channel borders. If several datasets have the same set of blank values, you don't need to call this function multiple times. When @code{aslinkedlist} is non-zero, then @code{input} will be seen as a @ref{List of gal_data_t} and for all the same neighbor position checking will be done for all the datasets in the list. Of course, the values for each dataset will be different, so a different value will be written in the each dataset, but the neighbor checking that is the most CPU intensive part will only be done once. @end deftypefun @node Git wrappers, Cosmology library, Interpolation, Gnuastro library @subsection Git wrappers (@file{git.h}) @cindex Git @cindex libgit2 Git is one of the most common tools for version control and it can often be useful during development, for example see @code{COMMIT} keyword in @ref{Output headers}. At installation time, Gnuastro will also check for the existence of libgit2, and store the value in the @code{GAL_CONFIG_HAVE_LIBGIT2}, see @ref{Configuration information} and @ref{Optional dependencies}. @file{gnuastro/git.h} includes @file{gnuastro/config.h} internally, so you won't have to include both for this macro. @deftypefun {char *} gal_git_describe ( ) When libgit2 is present and the program is called within a directory that is version controlled, this function will return a string containing the commit description (similar to Gnuastro's unofficial version number, see @ref{Version numbering}). If there are uncommitted changes in the running directory, it will add a `@code{-dirty}' prefix to the description. When there is no tagged point in the previous commit, this function will return a uniquely abbreviated commit object as fallback. This function is used for generating the value of the @code{COMMIT} keyword in @ref{Output headers}. The output string is similar to the output of the following command: @example $ git describe --dirty --always @end example Space for the output string is allocated within this function, so after using the value you have to @code{free} the output string. If libgit2 is not installed or the program calling this function is not within a version controlled directory, then the output will be the @code{NULL} pointer. @end deftypefun @node Cosmology library, , Git wrappers, Gnuastro library @subsection Cosmology library (@file{cosmology.h}) This library does the main cosmological calculations that are commonly necessary in extra-galactic astronomical studies. The main variable in this context is the redshift (@mymath{z}). The cosmological input parameters in the functions below are @code{H0}, @code{o_lambda_0}, @code{o_matter_0}, @code{o_radiation_0} which respectively represent the current (at redshift 0) expansion rate (Hubble constant in units of km/sec/Mpc), cosmological constant (@mymath{\Lambda}), matter and radiation densities. All these functions are declared in @file{gnuastro/cosmology.h}. For a more extended introduction/discussion of the cosmological parameters, please see @ref{CosmicCalculator}. @deftypefun double gal_cosmology_age (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Returns the age of the universe at redshift @code{z} in units of Giga years. @end deftypefun @deftypefun double gal_cosmology_proper_distance (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Returns the proper distance to an object at redshift @code{z} in units of Mega parsecs. @end deftypefun @deftypefun double gal_cosmology_comoving_volume (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Returns the comoving volume over 4pi stradian to @code{z} in units of Mega parsecs cube. @end deftypefun @deftypefun double gal_cosmology_critical_density (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Returns the critical density at redshift @code{z} in units of @mymath{g/cm^3}. @end deftypefun @deftypefun double gal_cosmology_angular_distance (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Return the angular diameter distance to an object at redshift @code{z} in units of Mega parsecs. @end deftypefun @deftypefun double gal_cosmology_luminosity_distance (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Return the luminosity diameter distance to an object at redshift @code{z} in units of Mega parsecs. @end deftypefun @deftypefun double gal_cosmology_distance_modulus (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Return the distance modulus at redshift @code{z} (with no units). @end deftypefun @deftypefun double gal_cosmology_to_absolute_mag (double @code{z}, double @code{H0}, double @code{o_lambda_0}, double @code{o_matter_0}, double @code{o_radiation_0}) Return the conversion from apparent to absolute magnitude for an object at redshift @code{z}. This value has to be added to the apparent magnitude to give the absolute magnitude of an object at redshift @code{z}. @end deftypefun @node Library demo programs, , Gnuastro library, Library @section Library demo programs In this final section of @ref{Library}, we give some example Gnuastro programs to demonstrate various features in the library. All these programs have been tested and once Gnuastro is installed you can compile and run them with with Gnuastro's @ref{BuildProgram} program that will take care of linking issues. If you don't have any FITS file to experiment on, you can use those that are generated by Gnuastro after @command{make check} in the @file{tests/} directory, see @ref{Quick start}. @menu * Library demo - reading a image:: Read a FITS image into memory. * Library demo - inspecting neighbors:: Inspect the neighbors of a pixel. * Library demo - multi-threaded operation:: Doing an operation on threads. * Library demo - reading and writing table columns:: Simple Column I/O. @end menu @node Library demo - reading a image, Library demo - inspecting neighbors, Library demo programs, Library demo programs @subsection Library demo - reading a FITS image The following simple program demonstrates how to read a FITS image into memory and use the @code{void *array} pointer in of @ref{Generic data container}. For easy linking/compilation of this program along with a first run see @ref{BuildProgram}. Before running, also change the @code{filename} and @code{hdu} variable values to specify an existing FITS file and/or extension/HDU. This is just intended to demonstrate how to use the @code{array} pointer of @code{gal_data_t}. Hence it doesn't do important sanity checks, for example in real datasets you may also have blank pixels. In such cases, this program will return a NaN value (see @ref{Blank pixels}). So for general statistical information of a dataset, it is much better to use Gnuastro's @ref{Statistics} program which can deal with blank pixels any many other issues in a generic dataset. @example #include #include #include /* includes gnuastro's data.h and type.h */ #include int main(void) @{ size_t i; float *farray; double sum=0.0f; gal_data_t *image; char *filename="img.fits", *hdu="1"; /* Read `img.fits' (HDU: 1) as a float32 array. */ image=gal_fits_img_read_to_type(filename, hdu, GAL_TYPE_FLOAT32, -1, 0, 0); /* Use the allocated space as a single precision floating * point array (recall that `image->array' has `void *' * type, so it is not directly usable. */ farray=image->array; /* Calculate the sum of all the values. */ for(i=0; isize; ++i) sum += farray[i]; /* Report the sum. */ printf("Sum of values in %s (hdu %s) is: %f\n", filename, hdu, sum); /* Clean up and return. */ gal_data_free(image); return EXIT_SUCCESS; @} @end example @node Library demo - inspecting neighbors, Library demo - multi-threaded operation, Library demo - reading a image, Library demo programs @subsection Library demo - inspecting neighbors The following simple program shows how you can inspect the neighbors of a pixel using the @code{GAL_DIMENSION_NEIGHBOR_OP} function-like macro that was introduced in @ref{Dimensions}. For easy linking/compilation of this program along with a first run see @ref{BuildProgram}. Before running, also change the file name and HDU (first and second arguments to @code{gal_fits_img_read_to_type}) to specify an existing FITS file and/or extension/HDU. @example #include #include #include int main(void) @{ double sum; float *array; size_t i, num, *dinc; gal_data_t *input=gal_fits_img_read_to_type("input.fits", "1", GAL_TYPE_FLOAT32, -1, 0, 0); /* To avoid the `void *' pointer and have `dinc'. */ array=input->array; dinc=gal_dimension_increment(input->ndim, input->dsize); /* Go over all the pixels. */ for(i=0;isize;++i) @{ num=0; sum=0.0f; GAL_DIMENSION_NEIGHBOR_OP( i, input->ndim, input->dsize, input->ndim, dinc, @{++num; sum+=array[nind];@} ); printf("%zu: num: %zu, sum: %f\n", i, num, sum); @} /* Clean up and return. */ gal_data_free(input); return EXIT_SUCCESS; @} @end example @node Library demo - multi-threaded operation, Library demo - reading and writing table columns, Library demo - inspecting neighbors, Library demo programs @subsection Library demo - multi-threaded operation The following simple program shows how to use Gnuastro to simplify spinning off threads and distributing different jobs between the threads. The relevant thread-related functions are defined in @ref{Gnuastro's thread related functions}. For easy linking/compilation of this program, along with a first run, see Gnuastro's @ref{BuildProgram}. Before running, also change the @code{filename} and @code{hdu} variable values to specify an existing FITS file and/or extension/HDU. This is a very simple program to open a FITS image, distribute its pixels between different threads and print the value of each pixel and the thread it was assigned to. The actual operation is very simple (and would not usually be done with threads in a real-life program). It is intentionally chosen to put more focus on the important steps in spinning of threads and how the worker function (which is called by each thread) can identify the job-IDs it should work on. For example, instead of an array of pixels, you can define an array of tiles or any other context-specific structures as separate targets. The important thing is that each action should have its own unique ID (counting from zero, as is done in an array in C). You can then follow the process below and use each thread to work on all the targets that are assigned to it. Recall that spinning-off threads is its self an expensive process and we don't want to spin-off one thread for each target (see the description of @code{gal_threads_dist_in_threads} in @ref{Gnuastro's thread related functions}. There are many (more complicated, real-world) examples of using @code{gal_threads_spin_off} in Gnuastro's actual source code, you can see them by searching for the @code{gal_threads_spin_off} function from the top source (after unpacking the tarball) directory (for example with this command): @example $ grep -r gal_threads_spin_off ./ @end example @noindent The code of this demonstration program is shown below. This program was also built and run when you ran @code{make check} during the building of Gnuastro (@code{tests/lib/multithread.c}, so it is already tested for your system and you can safely use it as a guide. @example #include #include #include "gnuastro/fits.h" #include "gnuastro/threads.h" /* This structure can keep all information you want to pass onto the * worker function on each thread. */ struct params @{ gal_data_t *image; /* Dataset to print values of. */ @}; /* This is the main worker function which will be called by the * different threads. `gal_threads_params' is defined in * `gnuastro/threads.h' and contains the pointer to the parameter we * want. Note that the input argument and returned value of this * function always must have `void *' type. */ void * worker_on_thread(void *in_prm) @{ /* Low-level definitions to be done first. */ struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct params *p=(struct params *)tprm->params; /* Subsequent definitions. */ float *array=p->image->array; size_t i, index, *dsize=p->image->dsize; /* Go over all the actions (pixels in this case) that were assigned * to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) @{ /* For easy reading. */ index = tprm->indexs[i]; /* Print the information. */ printf("(%zu, %zu) on thread %zu: %g\n", index%dsize[1]+1, index/dsize[1]+1, tprm->id, array[index]); @} /* Wait for all the other threads to finish, then return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; @} /* High-level function (called by the operating system). */ int main(void) @{ struct params p; char *filename="input.fits", *hdu="1"; size_t numthreads=gal_threads_number(); /* Read the image into memory as a float32 data type. We are using * `-1' for `minmapsize' to ensure that the image is read into * memory. */ p.image=gal_fits_img_read_to_type(filename, hdu, GAL_TYPE_FLOAT32, -1, 0, 0); /* Print some basic information before the actual contents: */ printf("Pixel values of %s (HDU: %s) on %zu threads.\n", filename, hdu, numthreads); printf("Used to check the compiled library's capability in opening " "a FITS file, and also spinning-off threads.\n"); /* A small sanity check: this is only intended for 2D arrays (to * print the coordinates of each pixel). */ if(p.image->ndim!=2) @{ fprintf(stderr, "only 2D images are supported."); exit(EXIT_FAILURE); @} /* Spin-off the threads and do the processing on each thread. */ gal_threads_spin_off(worker_on_thread, &p, p.image->size, numthreads); /* Clean up and return. */ gal_data_free(p.image); return EXIT_SUCCESS; @} @end example @node Library demo - reading and writing table columns, , Library demo - multi-threaded operation, Library demo programs @subsection Library demo - reading and writing table columns Tables are some of the most common inputs to, and outputs of programs. This section contains a small program for reading and writing tables using the constructs described in @ref{Table input output}. For easy linking/compilation of this program, along with a first run, see Gnuastro's @ref{BuildProgram}. Before running, also set the following file and column names in the first two lines of @code{main}. The input and output names may be @file{.txt} and @file{.fits} tables, @code{gal_table_read} and @code{gal_table_write} will be able to write to both formats. For plain text tables see see @ref{Gnuastro text table format}. This example program reads three columns from a table. The first two columns are selected by their name (@code{NAME1} and @code{NAME2}) and the third is selected by its number: column 10 (counting from 1). Gnuastro's column selection is discussed in @ref{Selecting table columns}. The first and second columns can be any type, but this program will convert them to @code{int32_t} and @code{float} for its internal usage respectively. However, the third column must be double for this program. So if it isn't, the program will abort with an error. Having the columns in memory, it will print them out along with their sum (just a simple application, you can do what ever you want at this stage). Reading the table finishes here. The rest of the program is a demonstration of writing a table. While parsing the rows, this program will change the first column (to be counters) and multiply the second by 10 (so the output will be different). Then it will define the order of the output columns by setting the @code{next} element (to create a @ref{List of gal_data_t}). Before writing, this function will also set names for the columns (units and comments can be defined in a similar manner). Writing the columns to a file is then done through a simple call to @code{gal_table_write}. The operations that are shown in this example program are not necessary all the time. For example, in many cases, you know the numerical data type of the column before writing your program (see @ref{Numeric data types}), so type checking and copying to a specific type won't be necessary. @example #include #include #include int main(void) @{ /* File names and column names (which may also be numbers). */ char *c1_name="NAME1", *c2_name="NAME2", *c3_name="10"; char *inname="input.fits", *hdu="1", *outname="out.fits"; /* Internal parameters. */ float *array2; double *array3; int32_t *array1; size_t i, counter=0; gal_data_t *c1, *c2; gal_data_t tmp, *col, *columns; gal_list_str_t *column_ids=NULL; /* Define the columns to read. */ gal_list_str_add(&column_ids, c1_name, 0); gal_list_str_add(&column_ids, c2_name, 0); gal_list_str_add(&column_ids, c3_name, 0); /* The columns were added in reverse, so correct it. */ gal_list_str_reverse(&column_ids); /* Read the desired columns. */ columns = gal_table_read(inname, hdu, column_ids, GAL_TABLE_SEARCH_NAME, 1, -1, NULL); /* Go over the columns, we'll assume that you don't know their type * a-priori, so we'll check */ counter=1; for(col=columns; col!=NULL; col=col->next) switch(counter++) @{ case 1: /* First column: we want it as int32_t. */ c1=gal_data_copy_to_new_type(col, GAL_TYPE_INT32); array1 = c1->array; break; case 2: /* Second column: we want it as float. */ c2=gal_data_copy_to_new_type(col, GAL_TYPE_FLOAT32); array2 = c2->array; break; case 3: /* Third column: it MUST be double. */ if(col->type!=GAL_TYPE_FLOAT64) @{ fprintf(stderr, "Column %s must be float64 type, it is " "%s", c3_name, gal_type_name(col->type, 1)); exit(EXIT_FAILURE); @} array3 = col->array; break; @} /* As an example application we'll just print them out. In the * meantime (just for a simple demonstration), change the first * array value to the counter and multiply the second by 10. */ for(i=0;isize;++i) @{ printf("%zu: %d + %f + %f = %f\n", i+1, array1[i], array2[i], array3[i], array1[i]+array2[i]+array3[i]); array1[i] = i+1; array2[i] *= 10; @} /* Link the first two columns as a list. */ c1->next = c2; c2->next = NULL; /* Set names for the columns and write them out. */ c1->name = "COUNTER"; c2->name = "VALUE"; gal_table_write(c1, NULL, GAL_TABLE_FORMAT_BFITS, outname); /* The names weren't allocated, so to avoid cleaning-up problems, * we'll set them to NULL. */ c1->name = c2->name = NULL; /* Clean up and return. */ gal_data_free(c1); gal_data_free(c2); gal_list_data_free(columns); gal_list_str_free(column_ids, 0); /* strings weren't allocated. */ return EXIT_SUCCESS; @} @end example @node Developing, Gnuastro programs list, Library, Top @chapter Developing The basic idea of GNU Astronomy Utilities is for an interested astronomer to be able to easily understand the code of any of the programs or libraries, be able to modify the code if s/he feels there is an improvement and finally, to be able to add new programs or libraries for their own benefit, and the larger community if they are willing to share it. In short, we hope that at least from the software point of view, the ``obscurantist faith in the expert's special skill and in his personal knowledge and authority'' can be broken, see @ref{Science and its tools}. With this aim in mind, Gnuastro was designed to have a very basic, simple, and easy to understand architecture for any interested inquirer. This chapter starts with very general design choices, in particular @ref{Why C} and @ref{Program design philosophy}. It will then get a little more technical about the Gnuastro code and file/directory structure in @ref{Coding conventions} and @ref{Program source}. @ref{The TEMPLATE program} discusses a minimal (and working) template to help in creating new programs or easier learning of a program's internal structure. Some other general issues about documentation, building and debugging are then discussed. This chapter concludes with how you can learn about the development and get involved in @ref{Gnuastro project webpage}, @ref{Developing mailing lists} and @ref{Contributing to Gnuastro}. @menu * Why C:: Why Gnuastro is designed in C. * Program design philosophy:: General ideas behind the package structure. * Coding conventions:: Gnuastro coding conventions. * Program source:: Conventions for the code. * Documentation:: Documentation is an integral part of Gnuastro. * Building and debugging:: Build and possibly debug during development. * Test scripts:: Understanding the test scripts. * Developer's checklist:: Checklist to finalize your changes. * Gnuastro project webpage:: Central hub for Gnuastro activities. * Developing mailing lists:: Stay up to date with Gnuastro's development. * Contributing to Gnuastro:: Share your changes with all users. @end menu @node Why C, Program design philosophy, Developing, Developing @section Why C programming language? @cindex C programming language @cindex C++ programming language @cindex Python programming language Currently the programming language that is most commonly used in scientific applications is C++@footnote{@url{https://isocpp.org/}}, Python@footnote{@url{https://www.python.org/}}, and Julia@footnote{@url{https://julialang.org/}} (which is a newcomer but swiftly gaining ground). One of the main reasons behind this choice is their high-level abstractions. However, GNU Astronomy Utilities is fully written in the C programming language@footnote{@url{https://en.wikipedia.org/wiki/C_(programming_language)}}. The reasons can be summarized with simplicity, portability and efficiency/speed. All three are very important in a scientific software and we will discuss them below. @cindex ANSI C @cindex ISO C90 @cindex Ritchie, Dennis @cindex Kernighan, Brian @cindex Stroustrup, Bjarne Simplicity can best be demonstrated in a comparison of the main books of C++ and C. The ``C programming language''@footnote{Brian Kernighan, Dennis Ritchie. @emph{The C programming language}. Prentice Hall, Inc., Second edition, 1988. It is also commonly known as K&R and is based on the ANSI C and ISO C90 standards.} book, written by the authors of C, is only 286 pages and covers a very good fraction of the language, it has also remained unchanged from 1988. C is the main programming language of nearly all operating systems and there is no plan of any significant update. On the other hand, the most recent ``C++ programming language''@footnote{Bjarne Stroustrup. @emph{The C++ programming language}. Addison-Wesley Professional; 4 edition, 2013.} book, also written by its author, has 1366 pages and its fourth edition came out in 2013! As discussed in @ref{Science and its tools}, it is very important for other scientists to be able to readily read the code of a program at their will with minimum requirements. @cindex Object oriented programming In C++, inheriting objects in the object oriented programming paradigm and their internal functions make the code very easy to write for a programmer who is deeply invested in those objects and understands all their relations well. But it simultaneously makes reading the program for a first time reader (a curious scientist who wants to know only how a small step was done) extremely hard. Before understanding the methods, the scientist has to invest a lot of time and energy in understanding those objects and their relations. But in C, everything is done with basic language types for example @code{int}s or @code{float}s and their pointers to define arrays. So when an outside reader is only interested in one part of the program, that part is all they have to understand. Recently it is also becoming common to write scientific software in Python, or a combination of it with C or C++. Python is a high level scripting language which doesn't need compilation. It is very useful when you want to do something on the go and don't want to be halted by the troubles of compiling, linking, memory checking, etc. When the datasets are small and the job is temporary, this ability of Python is great and is highly encouraged. A very good example might be plotting, in which Python is undoubtedly one of the best. But as the data sets increase in size and the processing becomes more complicated, the speed of Python scripts significantly decrease. So when the program doesn't change too often and is widely used in a large community, mostly on large data sets (like astronomical images), using Python will waste a lot of valuable research-hours. It is possible to wrap C or C++ functions with Python to fix the speed issue. But this creates further complexity, because the interested scientist has to master two programming languages and their connection (which is not trivial). Like C++, Python is object oriented, so as explained above, it needs a high level of experience with that particular program to reasonably understand its inner workings. To make things worse, since it is mainly for on-the-go programming@footnote{Note that Python is good for fast programming, not fast programs.}, it can undergo significant changes. One recent example is how Python 2.x and Python 3.x are not compatible. Lots of research teams that invested heavily in Python 2.x cannot benefit from Python 3.x or future versions any more. Some converters are available, but since they are automatic, lots of complications might arise in the conversion@footnote{For example see @url{https://arxiv.org/abs/1712.00461, Jenness (2017)} which describes how LSST is managing the transition.}. If a research project begins using Python 3.x today, there is no telling how compatible their investments will be when Python 4.x or 5.x will come out. This stems from the core principles of Python, which are very useful when you look in the `on the go' basis as described before and not future usage. Reproducibility (ability to run the code in the future) is a core principal of any scientific result, or the software that produced that result. Rebuilding all the dependencies of a software in an obsolete language is not easy. Future-proof code (as long as current operating systems will be used) is written in C. The portability of C is best demonstrated by the fact that both C++ and Python are part of the C-family of programming languages which also include Julia, Java, Perl, and many other languages. C libraries can be immediately included in C++, and it is easy to write wrappers for them in all C-family programming languages. This will allow other scientists to benefit from C libraries using any C-family language that they prefer. As a result, Gnuastro's library is already usable in C and C++, and wrappers will be@footnote{@url{http://savannah.gnu.org/task/?13786}} added for higher-level languages like Python, Julia and Java. @cindex Low level programming @cindex Programming, low level The final reason was speed. This is another very important aspect of C which is not independent of simplicity (first reason discussed above). The abstractions provided by the higher-level languages (which also makes learning them harder for a newcomer) comes at the cost of speed. Since C is a low-level language@footnote{Low-level languages are those that directly operate the hardware like assembly languages. So C is actually a high-level language, but it can be considered one of the lowest-level languages among all high-level languages.} (closer to the hardware), it is much less complex for both the human reader @emph{and} the computer. The benefits of simplicity for a human were discussed above. Simplicity for the computer translates into more efficiently (faster) programs. This creates a much closer relation between the scientist/programmer (or their program) and the actual data and processing. The GNU coding standards@footnote{@url{http://www.gnu.org/prep/standards/}} also encourage the use of C over all other languages when generality of usage and ``high speed'' is desired. @node Program design philosophy, Coding conventions, Why C, Developing @section Program design philosophy @cindex Gnulib The core processing functions of each program (and all libraries) are written mostly with the basic ISO C90 standard. We do make lots of use of the GNU additions to the C language in the GNU C library@footnote{Gnuastro uses many GNU additions to the C library. However, thanks to the GNU Portability library (Gnulib) which is included in the Gnuastro tarball, users of non-GNU/Linux operating systems can also benefit from all these features when using Gnuastro.}, but these functions are mainly used in the user interface functions (reading your inputs and preparing them prior to or after the analysis). The actual algorithms, which most scientists would be more interested in, are much more closer to ISO C90. For this reason, program source files that deal with user interface issues and those doing the actual processing are clearly separated, see @ref{Program source}. If anything particular to the GNU C library is used in the processing functions, it is explained in the comments in between the code. @cindex GNU Coreutils All the Gnuastro programs provide very low level and modular operations (modeled on GNU Coreutils). Almost all the basic command-line programs like @command{ls}, @command{cp} or @command{rm} on GNU/Linux operating systems are part of GNU Coreutils. This enables you to use shell scripting languages (for example GNU Bash) to operate on a large number of files or do very complex things through the creative combinations of these tools that the authors had never dreamed of. We have put a few simple examples in @ref{Tutorials}. @cindex @LaTeX{} @cindex GNU Bash @cindex Python Matplotlib @cindex Matplotlib, Python @cindex PGFplots in @TeX{} or @LaTeX{} For example all the analysis output can be saved as ASCII tables which can be fed into your favorite plotting program to inspect visually. Python's Matplotlib is very useful for fast plotting of the tables to immediately check your results. If you want to include the plots in a document, you can use the PGFplots package within @LaTeX{}, no attempt is made to include such operations in Gnuastro. In short, Bash can act as a glue to connect the inputs and outputs of all these various Gnuastro programs (and other programs) in any fashion. Of course, Gnuastro's programs are just front-ends to the main workhorse (@ref{Gnuastro library}), allowing a user to create their own programs (for example with @ref{BuildProgram}). So once the functions within programs become mature enough, they will be moved within the libraries for even more general applications. The advantage of this architecture is that the programs become small and transparent: the starting and finishing point of every program is clearly demarcated. For nearly all operations on a modern computer (fast file input-output) with a modest level of complexity, the read/write speed is insignificant compared to the actual processing a program does. Therefore the complexity which arises from sharing memory in a large application is simply not worth the speed gain. Gnuastro's design is heavily influenced from Eric Raymond's ``The Art of Unix Programming''@footnote{Eric S. Raymond, 2004, @emph{The Art of Unix Programming}, Addison-Wesley Professional Computing Series.} which beautifully describes the design philosophy and practice which lead to the success of Unix-based operating systems@footnote{KISS principle: Keep It Simple, Stupid!}. @node Coding conventions, Program source, Program design philosophy, Developing @section Coding conventions @cindex GNU coding standards @cindex Gnuastro coding convention In Gnuastro, we try our best to follow the GNU coding standards. Added to those, Gnuastro defines the following conventions. It is very important for readability that the whole package follows the same convention. @itemize @item The code must be easy to read by eye. So when the order of several lines within a function does not matter (for example when defining variables at the start of a function). You should put the lines in the order of increasing length and group the variables with similar types such that this half-pyramid of declarations becomes most visible. If the reader is interested, a simple search will show them the variable they are interested in. However, this visual aid greatly helps in general inspections of the code and help the reader get a grip of the function's processing. @item A function that cannot be fully displayed (vertically) in your monitor is probably too long and may be more useful if it is broken up into multiple functions. 40 lines is usually a good reference. When the start and end of a function are clearly visible in one glance, the function is much more easier to understand. This is most important for low-level functions (which usually define a lot of variables). Low-level functions do most of the processing, they will also be the most interesting part of a program for an inquiring astronomer. This convention is less important for higher level functions that don't define too many variables and whose only purpose is to run the lower-level functions in a specific order and with checks. @cindex Optimization flag @cindex GNU Compiler Collection In general you can be very liberal in breaking up the functions into smaller parts, the GNU Compiler Collection (GCC) will automatically compile the functions as inline functions when the optimizations are turned on. So you don't have to worry about decreasing the speed. By default Gnuastro will compile with the @option{-O3} optimization flag. @cindex Buffers (Emacs) @cindex Emacs buffers @item All Gnuastro hand-written text files (C source code, Texinfo documentation source, and version control commit messages) should not exceed @strong{75} characters per line. Monitors today are certainly much wider, but with this limit, reading the functions becomes much more easier. Also for the developers, it allows multiple files (or multiple views of one file) to be displayed beside each other on wide monitors. Emacs's buffers are excellent for this capability, setting a buffer width of 80 with `@key{C-u 80 C-x 3}' will allow you to view and work on several files or different parts of one file using the wide monitors common today. Emacs buffers can also be used as a shell prompt and compile the program (with @key{M-x compile}), and 80 characters is the default width in most terminal emulators. If you use Emacs, Gnuastro sets the 75 character @command{fill-column} variable automatically for you, see cartouche below. For long comments you can use press @key{Alt-q} in Emacs to separate them into separate lines automatically. For long literal strings, you can use the fact that in C, two strings immediately after each other are concatenated, for example @code{"The first part, " "and the second part."}. Note the space character in the end of the first part. Since they are now separated, you can easily break a long literal string into several lines and adhere to the maximum 75 character line length policy. @cindex Header file @item The headers required by each source file (ending with @file{.c}) should be defined inside of it. All the headers a complete program needs should @emph{not} be stacked in another header to include in all source files (for example @file{main.h}). Although most `professional' programmers choose this single header method, Gnuastro is primarily written for professional/inquisitive astronomers (who are generally amateur programmers). The list of header files included provides valuable general information and helps the reader. @file{main.h} may only include the header file(s) that define types that the main program structure needs, see @file{main.h} in @ref{Program source}. Those particular header files that are included in @file{main.h} can of course be ignored (not included) in separate source files. @item The headers should be classified (by an empty line) into separate groups: @enumerate @cindex GNU C library @cindex Gnulib: GNU Portability Library @cindex GNU Portability Library (Gnulib) @item @code{#include }: This must be the first code line (not commented or blank) in each source file @emph{within Gnuastro}. It sets macros that the GNU Portability Library (Gnulib) will use for a unified environment (GNU C Library), even when the user is building on a system that doesn't use the GNU C library. @item The C library header files, for example @file{stdio.h}, @file{stdlib.h}, or @file{math.h}. @item Installed library header files, including Gnuastro's installed headers (for example @file{cfitsio.h} or @file{gsl/gsl_rng.h}, or @file{gnuastro/fits.h}). @item Gnuastro's internal headers (that are not installed), for example @file{gnuastro-internal/options.h}. @item For programs, the @file{main.h} file (which is needed by the next group of headers). @item That particular program's header files, for example @file{mkprof.h}, or @file{noisechisel.h}. @end enumerate @noindent As much as order does not matter when you include the header of each group, sort them by length, as described above. @item All function names, variables, etc should be in lower case. Macros and constant global @code{enum}s should be in upper case. @item For the naming of exported header files, functions, variables, macros, and library functions, we adopt similar conventions to those used by the GNU Scientific Library (GSL)@footnote{@url{https://www.gnu.org/software/gsl/design/gsl-design.html#SEC15}}. In particular, in order to avoid clashes with the names of functions and variables coming from other libraries the name-space `@code{gal_}' is prefixed to them. GAL stands for @emph{G}NU @emph{A}stronomy @emph{L}ibrary. @item All installed header files should be in the @file{lib/gnuastro} directory (under the top Gnuastro source directory). After installation, they will be put in the @file{$prefix/include/gnuastro} directory (see @ref{Installation directory} for @file{$prefix}). Therefore with this convention Gnuastro's headers can be included in internal (to Gnuastro) and external (a library user) source files with the same line @example # include @end example Note that the GSL convention for header file names is @file{gsl_specialname.h}, so your include directive for a GSL header must be something like @code{#include }. Gnuastro doesn't follow this GSL guideline because of the repeated @code{gsl} in the include directive. It can be confusing and cause bugs for beginners. All Gnuastro (and GSL) headers must be located within a unique directory and will not be mixed with other headers. Therefore the `@file{gsl_}' prefix to the header file names is redundant@footnote{For GSL, this prefix has an internal technical application: GSL's architecture mixes installed and not-installed headers in the same directory. This prefix is used to identify their installation status. Therefore this filename prefix in GSL a technical internal issue (for developers, not users).}. @item @cindex GNU coding standards All installed functions and variables should also include the base-name of the file in which they are defined as prefix, using underscores to separate words@footnote{The convention to use underscores to separate words, called ``snake case'' (or ``snake_case''). This is also recommended by the GNU coding standards.}. The same applies to exported macros, but in upper case. For example in Gnuastro's top source directory, the prototype of function @code{gal_box_border_from_center} is in @file{lib/gnuastro/box.h}, and the macro @code{GAL_POLYGON_MAX_CORNERS} is defined in @code{lib/gnuastro/polygon.h}. This is necessary to give any user (who is not familiar with the library structure) the ability to follow the code. This convention does make the function names longer (a little harder to write), but the extra documentation it provides plays an important role in Gnuastro and is worth the cost. @item @cindex GNU Emacs @cindex Trailing space There should be no trailing white space in a line. To do this automatically every time you save a file in Emacs, add the following line to your @file{~/.emacs} file. @example (add-hook 'before-save-hook 'delete-trailing-whitespace) @end example @item @cindex Tabs are evil There should be no tabs in the indentation@footnote{If you use Emacs, Gnuastro's @file{.dir-locals.el} file will automatically never use tabs for indentation. To make this a default in all your Emacs sessions, you can add the following line to your @file{~/.emacs} file: @command{(setq-default indent-tabs-mode nil)}}. @item @cindex GNU Emacs @cindex Function groups @cindex Groups of similar functions Individual, contextually similar, functions in a source file are separated by 5 blank lines to be easily seen to be related in a group when parsing the source code by eye. In Emacs you can use @key{CTRL-u 5 CTRL-o}. @item One group of contextually similar functions in a source file is separated from another with 20 blank lines. In Emacs you can use @key{CTRL-u 20 CTRL-o}. Each group of functions has short descriptive title of the functions in that group. This title is surrounded by asterisks (@key{*}) to make it clearly distinguishable. Such contextual grouping and clear title are very important for easily understanding the code. @item Always read the comments before the patch of code under it. Similarly, try to add as many comments as you can regarding every patch of code. Effectively, we want someone to get a good feeling of the steps, without having to read the C code and only by reading the comments. This follows similar principles as @url{https://en.wikipedia.org/wiki/Literate_programming, Literate programming}. @end itemize The last two conventions are not common and might benefit from a short discussion here. With a good experience in advanced text editor operations, the last two are redundant for a professional developer. However, recall that Gnuastro aspires to be friendly to un-familiar, and un-experienced (in programming) eyes. In other words, as discussed in @ref{Science and its tools}, we want the code to appear welcoming to someone who is completely new to coding (and text editors) and only has a scientific curiosity. Newcomers to coding and development, who are curious enough to venture into the code, will probably not be using (or have any knowledge of) advanced text editors. They will see the raw code in the webpage or on a simple text editor (like Gedit) as plain text. Trying to learn and understand a file with dense functions that are all spaced with one or two blank lines can be very taunting for a newcomer. But when they scroll through the file and see clear titles and meaningful spaces for similar functions, we are helping them find and focus on the part they are most interested in sooner and easier. @cartouche @cindex GNU Emacs @noindent @strong{GNU Emacs, the recommended text editor:} GNU Emacs is an extensible and easily customizable text editor which many programmers rely on for developing due to its countless features. Among them, it allows specification of certain settings that are applied to a single file or to all files in a directory and its sub-directories. In order to harmonize code coming from different contributors, Gnuastro comes with a @file{.dir-locals.el} file which automatically configures Emacs to satisfy most of the coding conventions above when you are using it within Gnuastro's directories. Thus, Emacs users can readily start hacking into Gnuastro. If you are new to developing, we strongly recommend this editor. Emacs was the first project released by GNU and is still one of its flagship projects. Some resources can be found at: @table @asis @item Official manual At @url{https://www.gnu.org/software/emacs/manual/emacs.html}. This is a great and very complete manual which is being improved for over 30 years and is the best starting point to learn it. It just requires a little patience and practice, but rest assured that you will be rewarded. If you install Emacs, you also have access to this manual on the command-line with the following command (see @ref{Info}). @example $ info emacs @end example @item A guided tour of emacs At @url{https://www.gnu.org/software/emacs/tour/}. A short visual tour of Emacs, officially maintained by the Emacs developers. @item Unofficial mini-manual At @url{https://tuhdo.github.io/emacs-tutor.html}. A shorter manual which contains nice animated images of using Emacs. @end table @end cartouche @node Program source, Documentation, Coding conventions, Developing @section Program source @cindex Source file navigation @cindex Navigating source files @cindex Program structure convention @cindex Convention for program source @cindex Gnuastro program structure convention Besides the fact that all the programs share some functions that were explained in @ref{Library}, everything else about each program is completely independent. Recall that Gnuastro is written for an active astronomer/scientist (not a passive one who just uses a software). It must thus be easily navigable. Hence there are fixed source files (that contain fixed operations) that must be present in all programs, these are discussed fully in @ref{Mandatory source code files}. To easily understand the explanations in this section you can use @ref{The TEMPLATE program} which contains the bare minimum code for one working program. This template can also be used to easily add new utilities: just copy and paste the directory and change @code{TEMPLATE} with your program's name. @menu * Mandatory source code files:: Description of files common to all programs. * The TEMPLATE program:: Template for easy creation of a new program. @end menu @node Mandatory source code files, The TEMPLATE program, Program source, Program source @subsection Mandatory source code files Some programs might need lots of source files and if there is no fixed convention, navigating them can become very hard for a new inquirer into the code. The following source files exist in every program's source directory (which is located in @file{bin/progname}). For small programs, these files are enough. Larger programs will need more files and developers are encouraged to define any number of new files. It is just important that the following list of files exist and do what is described here. When creating other source files, please choose filenames that are a complete single word: don't abbreviate (abbreviations are cryptic). For a minimal program containing all these files, see @ref{The TEMPLATE program}. @vtable @file @item main.c @cindex @code{main} function Each executable has a @code{main} function, which is located in @file{main.c}. Therefore this file is the starting point when reading any program's source code. No actual processing functions must be defined in this file, the function(s) in this file are only meant to connect the most high level steps of each program. Generally, @code{main} will first call the top user interface function to read user input and make all the preparations. Then it will pass control to the top processing function for that program. The functions to do both these jobs must be defined in other source files. @item main.h @cindex Top root structure @cindex @code{prognameparams} @cindex Root parameter structure @cindex Main parameters C structure All the major parameters which will be used in the program must be stored in a structure which is defined in @file{main.h}. The name of this structure is usually @code{prognameparams}, for example @code{cropparams} or @code{noisechiselparams}. So @code{#include "main.h"} will be a staple in all the source codes of the program. It is also regularly the first (and only) argument most of the program's functions which greatly helps in readability. Keeping all the major parameters of a program in this structure has the major benefit that most functions will only need one argument: a pointer to this structure. This will significantly facilitate the job of the programmer, the inquirer and the computer. All the programs in Gnuastro are designed to be low-level, small and independent parts, so this structure should not get too large. @cindex @code{p} The main root structure of all programs contains at least one instance of the @code{gal_options_common_params} structure. This structure will keep the values to all common options in Gnuastro's programs (see @ref{Common options}). This top root structure is conveniently called @code{p} (short for parameters) by all the functions in the programs and the common options parameters within it are called @code{cp}. With this convention any reader can immediately understand where to look for the definition of one parameter. For example you know that @code{p->cp->output} is in the common parameters while @code{p->threshold} is in the program's parameters. @cindex Structure de-reference operator @cindex Operator, structure de-reference With this basic root structure, source code of functions can potentially become full of structure de-reference operators (@command{->}) which can make the code very un-readable. In order to avoid this, whenever a structure element is used more than a couple of times in a function, a variable of the same type and with the same name (so it can be searched) as the desired structure element should be defined with the value of the root structure inside of it in definition time. Here is an example. @example char *hdu=p->cp.hdu; float threshold=p->threshold; @end example @item args.h @cindex GNU C library @cindex Argp argument parser The options particular to each program are defined in this file. Each option is defined by a block of parameters in @code{program_options}. These blocks are all you should modify in this file, leave the bottom group of definitions untouched. These are fed directly into the GNU C library's Argp facilities and it is recommended to have a look at that for better understand what is going on, although this is not required here. Each element of the block defining an option is described under @code{argp_option} in @code{bootstrapped/lib/argp.h} (from Gnuastro's top source file). Note that the last few elements of this structure are Gnuastro additions (not documented in the standard Argp manual). The values to these last elements are defined in @code{lib/gnuastro/type.h} and @code{lib/gnuastro-internal/options.h} (from Gnuastro's top source directory). @item ui.h Besides declaring the exported functions of @code{ui.c}, this header also keeps the ``key''s to every program-specific option. The first class of keys for the options that have a short-option version (single letter, see @ref{Options}). The character that is defined here is the option's short option name. The list of available alphabet characters can be seen in the comments. Recall that some common options also take some characters, for those, see @file{lib/gnuastro-internal/options.h}. The second group of options are those that don't have a short option alternative. Only the first in this group needs a value (@code{1000}), the rest will be given a value by C's @code{enum} definition, so the actual value is irrelevant and must never be used, always use the name. @item ui.c @cindex User interface functions @cindex Functions for user interface Everything related to reading the user input arguments and options, checking the configuration files and checking the consistency of the input parameters before the actual processing is run should be done in this file. Since most functions are the same, with only the internal checks and structure parameters differing. We recommend going through the @code{ui.c} of @ref{The TEMPLATE program}, or several other programs for a better understanding. The most high-level function in @file{ui.c} is named @code{ui_read_check_inputs_setup}. It accepts the raw command-line inputs and a pointer to the root structure for that program (see the explanation for @file{main.h}). This is the function that @code{main} calls. The basic idea of the functions in this file is that the processing functions should need a minimum number of such checks. With this convention an inquirer who only wants to understand only one part (mostly the processing part and not user input details and sanity checks) of the code can easily do so in the later files. It also makes all the errors related to input appear before the processing begins which is more convenient for the user. @item progname.c, progname.h @cindex Top processing source file The high-level processing functions in each program are in a file named @file{progname.c}, for example @file{crop.c} or @file{noisechisel.c}. The function within these files which @code{main} calls is also named after the program, for example @example void crop(struct cropparams *p) @end example @noindent or @example void noisechisel(struct noisechiselparams *p) @end example @noindent In this manner, if an inquirer is interested the processing steps, they can immediately come and check this file for the first processing step without having to go through @file{main.c} and @file{ui.c} first. In most situations, any failure in any step of the programs will result in an informative error message and an immediate abort in the program. So there is usually no need for return values. Under more complicated situations where a return value might be necessary, @code{void} will be replaced with an @code{int} in the examples above. This value must be directly returned by @code{main}, so it has to be an @code{int}. @item authors-cite.h @cindex Citation information This header file keeps the global variable for the program authors and its BibTeX record for citation. They are used in the outputs of the common options @option{--version} and @option{--cite}, see @ref{Operating mode options}. @end vtable @node The TEMPLATE program, , Mandatory source code files, Program source @subsection The TEMPLATE program The extra creativity offered by libraries comes at a cost: you have to actually write your @code{main} function and get your hands dirty in managing user inputs: are all the necessary parameters given a value? is the input in the correct format? do the options and the inputs correspond? and many other similar checks. So when an operation has well-defined inputs and outputs and is commonly needed, it is much more worthwhile to simply do use all the great features that Gnuastro has already defined for such operations. To make it easier to learn/apply the internal program infra-structure discussed in @ref{Mandatory source code files}, Gnuastro ships with a template program when using the @ref{Version controlled source}. It is not available in the Gnuastro tarball so it doesn't confuse people using the tarball. The @file{bin/TEMPLATE} directory in Gnuastro's clone contains the bare-minimum files necessary to define a new program and all the necessary files/functions are pre-defined there. You can take the following steps if you want to add a new program to Gnuastro: @enumerate @item Select a name for your new program (for example @file{myprog}). @item Copy the @file{TEMPLATE} directory to a directory with your program's name: @example $ cp -R bin/TEMPLATE bin/myprog @end example @item Open @file{configure.ac} in the top Gnuastro source. This file manages the operations that are done when a user runs @file{./configure}. Going down the file, you will notice repetitive parts for each program. Copy one of those and correct the names of the copied program to your new program name. We follow alphabetic ordering here, so please place it correctly. There are multiple places where this has to be done, so be patient and go down to the bottom of the file. Ultimately add @file{bin/myprog/Makefile} to @code{AC_CONFIG_FILES}, only here the ordering depends on the length of the name. @item Open @file{Makefile.am} in the top Gnuastro source. Similar to the previous step, add your new program similar to all the other programs. @item Change @code{TEMPLATE} to @code{myprog} in the file names and contents of the files in the @file{bin/myprog/} directory. @item Run the following command to re-build the configuration and build system. @example $ autoreconf -f @end example Your new program will be built the next time you run @command{./configure} and @command{make}. You can now start adding your special checks/processing. @end enumerate @node Documentation, Building and debugging, Program source, Developing @section Documentation Documentation (this book) is an integral part of Gnuastro (see @ref{Science and its tools}). Documentation is not considered a separate project and must be written by its developers. Users can make edits/corrections, but the initial writing must be by the developer. So, no change is considered valid for implementation unless the respective parts of the book have also been updated. The following procedure can be a good suggestion to take when you have a new idea and are about to start implementing it. The steps below are not a requirement, the important thing is that when you send the program to be included in Gnuastro, the book and the code have to both be fully up-to-date and compatible and the purpose should be very clearly explained. You can follow any path you choose to do this, the following path was what we have found to be most successful until now. @enumerate @item Edit the book and fully explain your desired change, such that your idea is completely embedded in the general context of the book with no sense of discontinuity for a first time reader. This will allow you to plan the idea much more accurately and in the general context of Gnuastro or a particular program. Later on, when you are coding, this general context will significantly help you as a road-map. A very important part of this process is the program introduction, which explains the purposes of the program. Before actually starting to code, explain your idea's purpose thoroughly in the start of the program section you wish to add or edit. While actually writing its purpose for a new reader, you will probably get some very valuable ideas that you hadn't thought of before. This has occurred several times during the creation of Gnuastro. If an introduction already exists, embed or blend your idea's purpose with the existing purposes. We emphasize that doing this is equally useful for you (as the programmer) as it is useful for the user (reader). Recall that the purpose of a program is very important, see @ref{Program design philosophy}. As you have already noticed for every program, it is very important that the basics of the science and technique be explained in separate subsections prior to the `Invoking Programname' subsection. If you are writing a new program or your addition to an existing program involves a new concept, also include such subsections and explain the concepts so a person completely unfamiliar with the concepts can get a general initial understanding. You don't have to go deep into the details, just enough to get an interested person (with absolutely no background) started. If you feel you can't do that, then you have probably not understood the concept yourself! If you feel you don't have the time, then think about yourself as the reader in one year: you will forget almost all the details, so now that you have done all the theoretical preparations, add a few more hours and document it, so next time you don't have to prepare as much. Have in mind that your only limitation in length is the fatigue of the reader after reading a long text, nothing else. So as long as you keep it relevant/interesting for the reader, there is no page number limit/cost! It might also help if you start discussing the usage of your idea in the `Invoking ProgramName' subsection (explaining the options and arguments you have in mind) at this stage too. Actually starting to write it here will really help you later when you are coding. @item After you have finished adding your initial intended plan to the book, then start coding your change or new program within the Gnuastro source files. While you are coding, you will notice that somethings should be different from what you wrote in the book (your initial plan). So correct them as you are actually coding, but don't worry too much about missing a few things (see the next step). @item After your work has been fully implemented, read the section documentation from the start and see if you didn't miss any change in the coding and to see if the context is fairly continuous for a first time reader (who hasn't seen the book or had known Gnuastro before you made your change). @end enumerate @node Building and debugging, Test scripts, Documentation, Developing @section Building and debugging @cindex GNU Libtool @cindex GNU Autoconf @cindex GNU Automake @cindex GNU build system To build the various programs and libraries in Gnuastro, the GNU build system is used which defines the steps in @ref{Quick start}. It consists of GNU Autoconf, GNU Automake and GNU Libtool which are collectively known as GNU Autotools. They provide a very portable system to check the hosts environment and compile Gnuastro based on that. They also make installing everything in their standard places very easy for the programmer. Most of the small caps files that you see in the top source directory of the tarball are created by these three tools (see @ref{Version controlled source}). To facilitate the building and testing of your work during development, Gnuastro comes with two useful scripts: @table @file @cindex @file{tmpfs-config-make} @item tmpfs-config-make This is more fully described in @ref{Configure and build in RAM}. During development, you will usually run this command only once (at the start of your work). @cindex @file{tests/during-dev.sh} @item tests/during-dev.sh This script is designed to be run each time you make a change and want to test your work (with some possible input and output). The script itself is heavily commented and thoroughly describes the best way to use it, so we won't repeat it here. As a short summary: you specify the build directory, an output directory (for the built program to be run in, and also contains the inputs), the program's short name and the arguments and options that it should be run with. This script will then build Gnuastro, go to the output directory and run the built executable from there. One option for the output directory might be your desktop, so you can easily see the output files and delete them when you are finished. The main purpose of these scripts is to keep your source directory clean and facilitate your development. @end table @cindex Debugging @cindex Optimization By default all the programs are compiled with optimization flags for increased speed. A side effect of optimization is that valuable debugging information is lost. All the libraries are also linked as shared libraries by default. Shared libraries further complicate the debugging process and significantly slow down the compilation (the @command{make} command). So during development it is recommended to configure Gnuastro as follows: @example $ ./configure --disable-shared CFLAGS="-g -O0" @end example @noindent In @file{tmpfs-config-make} you can ask for this behavior by setting @code{debug_noshared} to @code{1}. In order to understand the building process, you can go through the Autoconf, Automake and Libtool manuals, like all GNU manuals they provide both a great tutorial and technical documentation. The ``A small Hello World'' section in Automake's manual (in chapter 2) can be a good starting guide after you have read the separate introductions. @node Test scripts, Developer's checklist, Building and debugging, Developing @section Test scripts @cindex Test scripts @cindex Gnuastro test scripts As explained in @ref{Tests}, for every program some simple tests are written to check the various independent features of the program. All the tests are placed in the @file{tests/} directory. The @file{tests/prepconf.sh} script is the first `test' that will be run. It will copy all the configuration files from the various directories to a @file{tests/.gnuastro} directory (which it will make) so the various tests can set the default values. This script will also make sure the programs don't go searching for user and system wide configuration files to avoid the mixing of values with different Gnuastro version on the system. For each program, the tests are placed inside directories with the program name. Each test is written as a shell script. The last line of this script is the test which runs the program with certain parameters. The return value of this script determines the fate of the test, see the ``Support for test suites'' chapter of the Automake manual for a very nice and complete explanation. In every script, two variables are defined at first: @code{prog} and @code{execname}. The first specifies the program name and the second the location of the executable. @cindex Build tree @cindex Source tree @cindex @file{tmpfs-config-make} The most important thing to have in mind about all the test scripts is that they are run from inside the @file{tests/} directory in the ``build tree''. Which can be different from the directory they are stored in (known as the ``source tree'')@footnote{The @file{tmpfs-config-make} script also uses this feature to keep the source and build directories separate (see @ref{Configure and build in RAM}).}. This distinction is made by GNU Autoconf and Automake (which configure, build and install Gnuastro) so that you can install the program even if you don't have write access to the directory keeping the source files. See the ``Parallel build trees (a.k.a VPATH builds)'' in the Automake manual for a nice explanation. Because of this, any necessary inputs that are distributed in the tarball@footnote{In many cases, the inputs of a test are outputs of previous tests, this doesn't apply to this class of inputs. Because all outputs of previous tests are in the ``build tree''.}, for example the catalogs necessary for checks in MakeProfiles and Crop, must be identified with the @command{$topsrc} prefix instead of @command{../} (for the top source directory that is unpacked). This @command{$topsrc} variable points to the source tree where the script can find the source data (it is defined in @file{tests/Makefile.am}). The executables and other test products were built in the build tree (where they are being run), so they don't need to be prefixed with that variable. This is also true for images or files that were produced by other tests. @node Developer's checklist, Gnuastro project webpage, Test scripts, Developing @section Developer's checklist This is a checklist of things to do after applying your changes/additions in Gnuastro: @enumerate @item If the change is non-trivial, write test(s) in the @file{tests/progname/} directory to test the change(s)/addition(s) you have made. Then add their file names to @file{tests/Makefile.am}. @item Run @command{$ make check} to make sure everything is working correctly. @item Make sure the documentation (this book) is completely up to date with your changes, see @ref{Documentation}. @item Commit the change to your issue branch (see @ref{Production workflow} and @ref{Forking tutorial}). Afterwards, run Autoreconf to generate the appropriate version number: @example $ autoreconf -f @end example @cindex Making a distribution package @item Finally, to make sure everything will be built, installed and checked correctly run the following command (after re-configuring, and re-building). To greatly speed up the process, use multiple threads (8 in the example below, change it appropriately) @example $ make distcheck -j8 @end example @noindent This command will create a distribution file (ending with @file{.tar.gz}) and try to compile it in the most general cases, then it will run the tests on what it has built in its own mini-environment. If @command{$ make distcheck} finishes successfully, then you are safe to send your changes to us to implement or for your own purposes. See @ref{Production workflow} and @ref{Forking tutorial}. @end enumerate @node Gnuastro project webpage, Developing mailing lists, Developer's checklist, Developing @section Gnuastro project webpage @cindex Bug @cindex Issue @cindex Tracker @cindex GNU Savannah @cindex Report a bug @cindex Management hub @cindex Feature request @cindex Central management @url{https://savannah.gnu.org/projects/gnuastro/, Gnuastro's central management hub}@footnote{@url{https://savannah.gnu.org/projects/gnuastro/}} is located on @url{https://savannah.gnu.org/, GNU Savannah}@footnote{@url{https://savannah.gnu.org/}}. Savannah is the central software development management system for many GNU projects. Through this central hub, you can view the list of activities that the developers are engaged in, their activity on the version controlled source, and other things. Each defined activity in the development cycle is known as an `issue' (or `item'). An issue can be a bug (see @ref{Report a bug}), or a suggested feature (see @ref{Suggest new feature}) or an enhancement or generally any @emph{one} job that is to be done. In Savannah, issues are classified into three categories or `tracker's: @table @asis @cindex Mailing list: bug-gnuastro @item Support This tracker is a way that (possibly anonymous) users can get in touch with the Gnuastro developers. It is a complement to the bug-gnuastro mailing list (see @ref{Report a bug}). Anyone can post an issue to this tracker. The developers will not submit an issue to this list. They will only reassign the issues in this list to the other two trackers if they are valid@footnote{Some of the issues registered here might be due to a mistake on the user's side, not an actual bug in the program.}. Ideally (when the developers have time to put on Gnuastro, please don't forget that Gnuastro is a volunteer effort), there should be no open items in this tracker. @item Bugs This tracker contains all the known bugs in Gnuastro (problems with the existing tools). @item Tasks The items in this tracker contain the future plans (or new features/capabilities) that are to be added to Gnuastro. @end table @noindent All the trackers can be browsed by a (possibly anonymous) visitor, but to edit and comment on the Bugs and Tasks trackers, you have to be a registered on Savannah. When posting an issue to a tracker, it is very important to choose the `Category' and `Item Group' options accurately. The first contains a list of all Gnuastro's programs along with `Installation', `New program' and `Webpage'. The ``Item Group'' contains the nature of the issue, for example if it is a `Crash' in the software (a bug), or a problem in the documentation (also a bug) or a feature request or an enhancement. The set of horizontal links on the top of the page (Starting with `Main' and `Homepage' and finishing with `News') are the easiest way to access these trackers (and other major aspects of the project) from any part of the project webpage. Hovering your mouse over them will open a drop down menu that will link you to the different things you can do on each tracker (for example, `Submit new' or `Browse'). When you browse each tracker, you can use the ``Display Criteria'' link above the list to limit the displayed issues to what you are interested in. The `Category' and `Group Item' (explained above) are a good starting point. @cindex Mailing list: gnuastro-devel Any new issue that is submitted to any of the trackers, or any comments that are posted for an issue, is directly forwarded to the gnuastro-devel mailing list (@url{https://lists.gnu.org/mailman/listinfo/gnuastro-devel}, see @ref{Developing mailing lists} for more). This will allow anyone interested to be up to date on the over-all development activity in Gnuastro and will also provide an alternative (to Savannah) archiving for the development discussions. Therefore, it is not recommended to directly post an email to this mailing list, but do all the activities (for example add new issues, or comment on existing ones) on Savannah. @cartouche @noindent @strong{Do I need to be a member in Savannah to contribute to Gnuastro?} No. The full version controlled history of Gnuastro is available for anonymous download or cloning. See @ref{Production workflow} for a description of Gnuastro's Integration-Manager Workflow. In short, you can either send in patches, or make your own fork. If you choose the latter, you can push your changes to your own fork and inform us. We will then pull your changes and merge them into the main project. Please see @ref{Forking tutorial} for a tutorial. @end cartouche @node Developing mailing lists, Contributing to Gnuastro, Gnuastro project webpage, Developing @section Developing mailing lists To keep the developers and interested users up to date with the activity and discussions within Gnuastro, there are two mailing lists which you can subscribe to: @table @asis @item @command{gnuastro-devel@@gnu.org} @itemx (at @url{https://lists.gnu.org/mailman/listinfo/gnuastro-devel}) @cindex Mailing list: gnuastro-devel All the posts made in the support, bugs and tasks discussions of @ref{Gnuastro project webpage} are also sent to this mailing address and archived. By subscribing to this list you can stay up to date with the discussions that are going on between the developers before, during and (possibly) after working on an issue. All discussions are either in the context of bugs or tasks which are done on Savannah and circulated to all interested people through this mailing list. Therefore it is not recommended to post anything directly to this mailing list. Any mail that is sent to it from Savannah to this list has a link under the title ``Reply to this item at:''. That link will take you directly to the issue discussion page, where you can read the discussion history or join it. While you are posting comments on the Savannah issues, be sure to update the meta-data. For example if the task/bug is not assigned to anyone and you would like to take it, change the ``Assigned to'' box, or if you want to report that it has been applied, change the status and so on. All these changes will also be circulated with the email very clearly. @item @command{gnuastro-commits@@gnu.org} @itemx (at @url{https://lists.gnu.org/mailman/listinfo/gnuastro-commits}) @cindex Mailing list: gnuastro-commits This mailing list is defined to circulate all commits that are done in Gnuastro's version controlled source, see @ref{Version controlled source}. If you have any ideas, or suggestions on the commits, please use the bug and task trackers on Savannah to followup the discussion, do not post to this list. All the commits that are made for an already defined issue or task will state the respective ID so you can find it easily. @end table @node Contributing to Gnuastro, , Developing mailing lists, Developing @section Contributing to Gnuastro You have this great idea or have found a good fix to a problem which you would like to implement in Gnuastro. You have also become familiar with the general design of Gnuastro in the previous sections of this chapter (see @ref{Developing}) and want to start working on and sharing your new addition/change with the whole community as part of the official release. This is great and your contribution is most welcome. This section and the next (see @ref{Developer's checklist}) are written in the hope of making it as easy as possible for you to share your great idea with the community. @cindex FSF @cindex Free Software Foundation In this section we discuss the final steps you have to take: legal and technical. From the legal perspective, the copyright of any work you do on Gnuastro has to be assigned to the Free Software Foundation (FSF) and the GNU operating system, or you have to sign a disclaimer. We do this to ensure that Gnuastro can remain free in the future, see @ref{Copyright assignment}. From the technical point of view, in this section we also discuss commit guidelines (@ref{Commit guidelines}) and the general version control workflow of Gnuastro in @ref{Production workflow}, along with a tutorial in @ref{Forking tutorial}. Recall that before starting the work on your idea, be sure to checkout the bugs and tasks trackers in @ref{Gnuastro project webpage} and announce your work there so you don't end up spending time on something others have already worked on, and also to attract similarly interested developers to help you. @menu * Copyright assignment:: Copyright has to be assigned to the FSF. * Commit guidelines:: Guidelines for commit messages. * Production workflow:: Submitting your commits (work) for inclusion. * Forking tutorial:: Tutorial on workflow steps with Git. @end menu @node Copyright assignment, Commit guidelines, Contributing to Gnuastro, Contributing to Gnuastro @subsection Copyright assignment Gnuastro's copyright is owned by the FSF. Professor Eben Moglen, of the Columbia University Law School has given a nice summary of the reasons for this at @url{https://www.gnu.org/licenses/why-assign}. Below we are copying it verbatim for self consistency (in case you are offline or reading in print). @quotation Under US copyright law, which is the law under which most free software programs have historically been first published, there are very substantial procedural advantages to registration of copyright. And despite the broad right of distribution conveyed by the GPL, enforcement of copyright is generally not possible for distributors: only the copyright holder or someone having assignment of the copyright can enforce the license. If there are multiple authors of a copyrighted work, successful enforcement depends on having the cooperation of all authors. In order to make sure that all of our copyrights can meet the record keeping and other requirements of registration, and in order to be able to enforce the GPL most effectively, FSF requires that each author of code incorporated in FSF projects provide a copyright assignment, and, where appropriate, a disclaimer of any work-for-hire ownership claims by the programmer's employer. That way we can be sure that all the code in FSF projects is free code, whose freedom we can most effectively protect, and therefore on which other developers can completely rely. @end quotation Please get in touch with the Gnuastro maintainer (currently Mohammad Akhlaghi, akhlaghi -at- gnu -dot- org) to follow the procedures. It is possible to do this for each change (good for for a single contribution), and also more generally for all the changes/additions you do in the future within Gnuastro. So if you have already assigned the copyright of your work on another GNU software to the FSF, it should be done again for Gnuastro. The FSF has staff working on these legal issues and the maintainer will get you in touch with them to do the paperwork. The maintainer will just be informed in the end so your contributions can be merged within the Gnuastro source code. Gnuastro will gratefully acknowledge (see @ref{Acknowledgments}) all the people who have assigned their copyright to the FSF and have thus helped to guarantee the freedom and reliability of Gnuastro. The Free Software Foundation will also acknowledge your copyright contributions in the Free Software Supporter: @url{https://www.fsf.org/free-software-supporter} which will circulate to a very large community (104,444 people in April 2016). See the archives for some examples and subscribe to receive interesting updates. The very active code contributors (or developers) will also be recognized as project members on the Gnuastro project webpage (see @ref{Gnuastro project webpage}) and can be given a @code{gnu.org} email address. So your very valuable contribution and copyright assignment will not be forgotten and is highly appreciated by a very large community. If you are reluctant to sign an assignment, a disclaimer is also acceptable. @cartouche @noindent @strong{Do I need a disclaimer from my university or employer?} It depends on the contract with your university or employer. From the FSF's @file{/gd/gnuorg/conditions.text}: ``If you are employed to do programming, or have made an agreement with your employer that says it owns programs you write, we need a signed piece of paper from your employer disclaiming rights to'' Gnuastro. The FSF's copyright clerk will kindly help you decide, please consult the following email address: ``assign -at- gnu -dot- org''. @end cartouche @node Commit guidelines, Production workflow, Copyright assignment, Contributing to Gnuastro @subsection Commit guidelines To be able to cleanly integrate your work with the other developers, @strong{never commit on the @file{master} branch} (see @ref{Production workflow} for a complete discussion and @ref{Forking tutorial} for a cookbook example). In short, leave @file{master} only for changes you fetch, or pull from the official repository (see @ref{Synchronizing}). In the Gnuastro commit messages, we strive to follow these standards. Note that in the early phases of Gnuastro's development, we are experimenting and so if you notice earlier commits don't satisfy some of the guidelines below, it is because they predate that guideline. @table @asis @item Commit title The commits have to start with one short descriptive title. The title is separated from the body with one blank line. Run @command{git log} to see some of the most recent commit messages as an example. In general, the title should satisfy the following conditions: @itemize @item It is best for the title to be short, about 60 (or even 50) characters. Most emulated command-line terminals are about 80 characters wide. However, we should also allow for the commit hashes which are printed in @command{git log --oneline}, and also branch names or the graph structure outputs of @command{git log} which are also commonly used. @item The title should not finish with any full-stops or periods (`@key{.}'). @end itemize @item Commit body @cindex Mailing list: gnuastro-commits The body of the commit message is separated from the title by one empty line. Recall that anyone who has subscribed to @command{gnuastro-commits} mailing list will get the commit in their email after it has been pushed to @file{master}. People will also read them when they synchronize with the main Gnuastro repository (see @ref{Synchronizing}). Finally, the commit messages will later be used to update the @file{NEWS} file on each release. Therefore the commit message body plays a very important role in the development of Gnuastro, so please adhere to the following guidelines. @itemize @item The body should be very descriptive. Start the commit message body by explaining what changes your commit makes from a user's perspective (added, changed, or removed options, or arguments to programs or libraries, or modified algorithms, or new installation step, or etc). @item @cindex Mailing list: gnuastro-commits Try to explain the committed contents as best as you can. Recall that the readers of your commit message do not necessarily have your current background. After some time you will also forget the context, so this request is not just for others@footnote{@url{http://catb.org/esr/writings/unix-koans/prodigy.html}}. Therefore be very descriptive and explain as much as possible: what the bug/task was, justify the way you fixed it and discuss other possible solutions that you might not have included. For the last item, it is best to discuss them thoroughly as comments in the appropriate section of the code, but only give a short summary in the commit message. Note that all added and removed source code lines will also be circulated in the @command{gnuastro-commits} mailing list. @item Like all other Gnuastro's text files, the lines in the commit body should not be longer than 75 characters, see @ref{Coding conventions}. This is to ensure that on standard terminal emulators (with 80 character width), the @command{git log} output can be cleanly displayed (note that the commit message is indented in the output of @command{git log}). If you use Emacs, Gnuastro's @file{.dir-locals.el} file will ensure that your commits satisfy this condition (using @key{M-q}). @item @cindex Mailing list: gnuastro-commits When the commit is related to a task or a bug, please include the respective ID (in the format of @code{bug/task #ID}, note the space) in the commit message (from @ref{Gnuastro project webpage}) for interested people to be able to followup the discussion that took place there. If the commit fixes a bug or finishes a task, the recommended way is to add a line after the body with `@code{This fixes bug #ID.}', or `@code{This finishes task #ID.}'. Don't assume that the reader has internet access to check the bug's full description when reading the commit message, so give a short introduction too. @end itemize @end table @node Production workflow, Forking tutorial, Commit guidelines, Contributing to Gnuastro @subsection Production workflow Fortunately `Pro Git' has done a wonderful job in explaining the different workflows in Chapter 5@footnote{@url{http://git-scm.com/book/en/v2/Distributed-Git-Distributed-Workflows}} and in particular the ``Integration-Manager Workflow'' explained there. The implementation of this workflow is nicely explained in Section 5.2@footnote{@url{http://git-scm.com/book/en/v2/Distributed-Git-Contributing-to-a-Project}} under ``Forked-Public-Project''. We have also prepared a short tutorial in @ref{Forking tutorial}. Anything on the master branch should always be tested and ready to be built and used. As described in `Pro Git', there are two methods for you to contribute to Gnuastro in the Integration-Manager Workflow: @enumerate @item You can send commit patches by email as fully explained in `Pro Git'. This is good for your first few contributions. Just note that raw patches (containing only the diff) do not have any meta-data (author name, date and etc). Therefore they will not allow us to fully acknowledge your contributions as an author in Gnuastro: in the @file{AUTHORS} file and at the start of the PDF book. These author lists are created automatically from the version controlled source. To receive full acknowledgment when submitting a patch, is thus advised to use Git's @code{format-patch} tool. See Pro Git's @url{https://git-scm.com/book/en/v2/Distributed-Git-Contributing-to-a-Project#Public-Project-over-Email, Public project over email} section for a nice explanation. If you would like to get more heavily involved in Gnuastro's development, then you can try the next solution. @item You can have your own forked copy of Gnuastro on any hosting site you like (GitHub, GitLab, BitBucket, or etc) and inform us when your changes are ready so we merge them in Gnuastro. This is more suited for people who commonly contribute to the code (see @ref{Forking tutorial}). @end enumerate In both cases, your commits (with your name and information) will be preserved and your contributions will thus be fully recorded in the history of Gnuastro and in the @file{AUTHORS} file and this book (second page in the PDF format) once they have been incorporated into the official repository. Needless to say that in such cases, be sure to follow the bug or task trackers (or subscribe to the @command{gnuastro-devel} mailing list) and contact us before hand so you don't do something that someone else is already working on. In that case, you can get in touch with them and help the job go on faster, see @ref{Gnuastro project webpage}. This workflow is currently mostly borrowed from the general recommendations of Git@footnote{@url{https://github.com/git/git/blob/master/Documentation/SubmittingPatches}} and GitHub. But since Gnuastro is currently under heavy development, these might change and evolve to better suit our needs. @node Forking tutorial, , Production workflow, Contributing to Gnuastro @subsection Forking tutorial This is a tutorial on the second suggested method (commonly known as forking) that you can submit your modifications in Gnuastro (see @ref{Production workflow}). To start, please create an empty repository on your hosting service webpage (we recommend GitLab@footnote{See @url{https://www.gnu.org/software/repo-criteria-evaluation.html} for an evaluation of the major existing repositories. Gnuastro uses GNU Savannah (which also has the highest ranking in the evaluation), but for starters, GitLab may be easier.}). If this is your first hosted repository on the webpage, you also have to upload your public SSH key@footnote{For example see this explanation provided by GitLab: @url{http://docs.gitlab.com/ce/ssh/README.html}.} for the @command{git push} command below to work. Here we'll assume you use the name @file{janedoe} to refer to yourself everywhere and that you choose @file{gnuastro-janedoe} as the name of your Gnuastro fork. Any online hosting service will give you an address (similar to the `@file{git@@gitlab.com:...}' below) of the empty repository you have created using their webpage, use that address in the third line below. @example $ git clone git://git.sv.gnu.org/gnuastro.git $ cd gnuastro $ git remote add janedoe git@@gitlab.com:janedoe/gnuastro-janedoe.git $ git push janedoe master @end example The full Gnuastro history is now pushed onto your hosting service and the @file{janedoe} remote is now also following your @file{master} branch. If you run @command{git remote show REMOTENAME} for the @file{origin} and @file{janedoe} remotes, you will see their difference: the first has pull access and the second doesn't. This nicely summarizes the main idea behind this workflow: you push to your remote repository, we pull from it and merge it into @file{master}, then you finalize it by pulling from the main repository. To test (compile) your changes during your work, you will need to bootstrap the version controlled source, see @ref{Bootstrapping} for a full description. The cloning process above is only necessary for your first time setup, you don't need to repeat it. However, please repeat the steps below for each independent issue you intend to work on. Let's assume you have found a bug in @file{lib/statistics.c}'s median calculating function. Before actually doing anything, please announce it (see @ref{Report a bug}) so everyone knows you are working on it or to find out others aren't already working on it. With the commands below, you make a branch, checkout to it, correct the bug, check if it is indeed fixed, add it to the staging area, commit it to the new branch and push it to your hosting service. But before all of them, make sure that you are on the @file{master} branch and that your @file{master} branch is up to date with the main Gnuastro repository with the first two commands. @example $ git checkout master $ git pull $ git checkout -b bug-median-stats # Choose a descriptive name $ emacs lib/statistics.c $ # do your checks here $ git add lib/statistics.c $ git commit $ git push janedoe bug-median-stats @end example Your new branch is now on your hosted repository. Through the respective tacker on Savannah (see @ref{Gnuastro project webpage}) you can then let the other developers know that your @file{bug-median-stats} branch is ready. They will pull your work, test it themselves and if it is ready to be merged into the main Gnuastro history, they will merge it into the @file{master} branch. After that is done, you can simply checkout your local @file{master} branch and pull all the changes from the main repository. After the pull you can run `@command{git log}' as shown below, to see how @file{bug-median-stats} is merged with master. To finalize, you can push all the changes to your hosted repository and delete the branch: @example $ git checkout master $ git pull $ git log --oneline --graph --decorate --all $ git push janedoe master $ git branch -d bug-median-stats # delete local branch $ git push janedoe --delete bug-median-stats # delete remote branch @end example Just as a reminder, always keep your work on each issue in a separate local and remote branch so work can progress on them independently. After you make your announcement, other people might contribute to the branch before merging it in to @file{master}, so this is very important. As a final reminder: before starting each issue branch from @file{master}, be sure to run @command{git pull} in @file{master} as shown above. This will enable you to start your branch (work) from the most recent commit and thus simplify the final merging of your work. @node Gnuastro programs list, Other useful software, Developing, Top @appendix Gnuastro programs list GNU Astronomy Utilities @value{VERSION}, contains the following programs. They are sorted in alphabetical order and a short description is provided for each program. The description starts with the executable names in @file{thisfont} followed by a pointer to the respective section in parenthesis. Throughout this book, they are ordered based on their context, please see the top-level contents for contextual ordering (based on what they do). @table @asis @item Arithmetic (@file{astarithmetic}, see @ref{Arithmetic}) For arithmetic operations on multiple (theoretically unlimited) number of datasets (images). It has a large and growing set of arithmetic, mathematical, and even statistical operators (for example @command{+}, @command{-}, @command{*}, @command{/}, @command{sqrt}, @command{log}, @command{min}, @command{average}, @command{median}). @item BuildProgram (@file{astbuildprog}, see @ref{BuildProgram}) Compile, link and run programs that depend on the Gnuastro library (see @ref{Gnuastro library}). This program will automatically link with the libraries that Gnuastro depends on, so there is no need to explicitly mention them every time you are compiling a Gnuastro library dependent program. @item ConvertType (@file{astconvertt}, see @ref{ConvertType}) Convert astronomical data files (FITS or IMH) to and from several other standard image and data formats, for example TXT, JPEG, EPS or PDF. @item Convolve (@file{astconvolve}, see @ref{Convolve}) Convolve (blur or smooth) data with a given kernel in spatial and frequency domain on multiple threads. Convolve can also do de-convolution to find the appropriate kernel to PSF-match two images. @item CosmicCalculator (@file{astcosmiccal}, see @ref{CosmicCalculator}) Do cosmological calculations, for example the luminosity distance, distance modulus, comoving volume and many more. @item Crop (@file{astcrop}, see @ref{Crop}) Crop region(s) from an image and stitch several images if necessary. Inputs can be in pixel coordinates or world coordinates. @item Fits (@file{astfits}, see @ref{Fits}) View and manipulate FITS file extensions and header keywords. @item Statistics (@file{aststatistics}, see @ref{Statistics}) Get pixel statistics and save histogram and cumulative frequency plots. @item MakeCatalog (@file{astmkcatalog}, see @ref{MakeCatalog}) Make catalog of labeled image (output of NoiseChisel). The catalogs are highly customizable and adding new calculations/columns is very straightforward. @item MakeNoise (@file{astmknoise}, see @ref{MakeNoise}) Make (add) noise to an image, with a large set of random number generators and any seed. @item MakeProfiles (@file{astmkprof}, see @ref{MakeProfiles}) Make mock 2D profiles in an image. The central regions of radial profiles are made with a configurable 2D Monte Carlo integration. It can also build the profiles on an over-sampled image. @item Match (@file{astmatch}, see @ref{Match}) Given two input catalogs, find the rows that match with each other within a given aperture (may be an ellipse). @item NoiseChisel (@file{astnoisechisel}, see @ref{NoiseChisel}) Detect and segment signal in noise. It uses a technique to detect very faint and diffuse, irregularly shaped signal in noise (galaxies in the sky), using thresholds that are below the Sky value, see @url{http://arxiv.org/abs/1505.01664, arXiv:1505.01664}. @item Table (@file{asttable}, @ref{Table}) Convert FITS binary and ASCII tables into other such tables, print them on the command-line, save them in a plain text file, or get the FITS table information. @item Warp (@file{astwarp}, see @ref{Warp}) Warp image to new pixel grid. Any projective transformation or Homography can be applied to the input images. @end table @node Other useful software, GNU Free Doc. License, Gnuastro programs list, Top @appendix Other useful software In this appendix the installation of programs and libraries that are not direct Gnuastro dependencies are discussed. However they can be useful for working with Gnuastro. @menu * SAO ds9:: Viewing FITS images. * PGPLOT:: Plotting directly in C @end menu @node SAO ds9, PGPLOT, Other useful software, Other useful software @section SAO ds9 @cindex SAO ds9 @cindex FITS image viewer SAO ds9@footnote{@url{http://ds9.si.edu/}} is not a requirement of Gnuastro, it is a FITS image viewer. So to check your inputs and outputs, it is one of the best options. Like the other packages, it might already be available in your distribution's repositories. It is already pre-compiled in the download section of its webpage. Once you download it you can unpack and install (move it to a system recognized directory) with the following commands (@code{x.x.x} is the version number): @example $ tar xf ds9.linux64.x.x.x.tar.gz $ sudo mv ds9 /usr/local/bin @end example Once you run it, there might be a complaint about the Xss library, which you can find in your distribution package management system. You might also get an @command{XPA} related error. In this case, you have to add the following line to your @file{~/.bashrc} and @file{~/.profile} file (you will have to log out and back in again for the latter): @example export XPA_METHOD=local @end example @menu * Viewing multiextension FITS images:: Configure SAO ds9 for multiextension images. @end menu @node Viewing multiextension FITS images, , SAO ds9, SAO ds9 @subsection Viewing multiextension FITS images @cindex Multiextension FITS @cindex Opening multiextension FITS The FITS definition allows for multiple extensions inside a FITS file, each extension can have a completely independent data set inside of it. If you ordinarily open a multi-extension FITS file with SAO ds9, for example by double clicking on the file or running @command{$ds9 foo.fits}, SAO ds9 will only show you the first extension. To be able to switch between the extensions you have to follow these menus in the SAO ds9 window: @clicksequence{File@click{}Open Other@click{}Open Multi Ext Cube} and then choose the Multi extension FITS file in your computer's file structure. @cindex @option{-mecube} (ds9) The method above is a little tedious to do every time you want view a multi-extension FITS file. Fortunately SAO ds9 also provides options that you can use to specify a particular behavior. One of those options is @option{-mecube} which opens a FITS image as a multi-extension data cube. So on the command-line, if you run @command{$ds9 -mecube foo.fits} a small window will also be opened, which allows you to switch between the image extensions that @file{foo.fits} might have. If @file{foo.fits} only consists of one extension, then SAO ds9 will open as usual. Just to avoid confusion, note that SAO ds9 does not follow the GNU style of separating long and short options as explained in @ref{Arguments and options}. In the GNU style, this `long' option should have been called like @option{--mecube}, but SAO ds9 does follow those conventions and has its own. @cindex GNOME 3 It is really convenient if you set ds9 to always run with the @option{-mecube} option on your graphical display. On GNOME 3 (the most popular graphic user interface for GNU/Linux systems) you can do this by taking the following steps: @itemize @item @cindex @file{.desktop} Open your favorite text editor and put the following text in a file that ends with @file{.desktop}, for example @file{saods9.desktop}. The file is very descriptive. @example [Desktop Entry] Type=Application Version=1.0 Name=SAO ds9 Comment=View FITS images Exec=ds9 -mecube %f Terminal=false Categories=Graphic;FITS; @end example @item Copy this file into your local (user) applications directory: @example $ cp saods9.desktop ~/.local/share/applications/ @end example In case you don't have the directory, you can make it yourself: @example $ mkdir -p ~/.local/share/applications/ @end example @item The steps above will add SAO ds9 as one of your applications. To make it default for every time you click on a FITS file. Right click on a FITS file and select ``Open With'', then go into ``Other Application...'' and choose ``SAO ds9''. @end itemize @cindex GNOME 2 In case you are using GNOME 2 you can take the following steps: right click on a FITS file and choose @clicksequence{Properties@click{}Open With@click{}Add} button. A list of applications will show up, ds9 might already be present in the list, but don't choose it because it will run with no options. Below the list is an option ``Use a custom command''. Click on it and write the following command: @command{ds9 -mecube} in the box and click ``Add''. Then finally choose the command you just added as the default and click the ``Close'' button. @node PGPLOT, , SAO ds9, Other useful software @section PGPLOT @cindex PGPLOT @cindex C, plotting @cindex Plotting directly in C PGPLOT is a package for making plots in C. It is not directly needed by Gnuastro, but can be used by WCSLIB, see @ref{WCSLIB}. As explained in @ref{WCSLIB}, you can install WCSLIB without it too. It is very old (the most recent version was released early 2001!), but remains one of the main packages for plotting directly in C. WCSLIB uses this package to make plots if you want it to make plots. If you are interested you can also use it for your own purposes. @cindex Python Matplotlib @cindex Matplotlib, Python @cindex PGFplots in @TeX{} or @LaTeX{} If you want your plotting codes in between your C program, PGPLOT is currently one of your best options. The recommended alternative to this method is to get the raw data for the plots in text files and input them into any of the various more modern and capable plotting tools separately, for example the Matplotlib library in Python or PGFplots in @LaTeX{}. This will also significantly help code readability. Let's get back to PGPLOT for the sake of WCSLIB. Installing it is a little tricky (mainly because it is so old!). You can download the most recent version from the FTP link in its webpage@footnote{@url{http://www.astro.caltech.edu/~tjp/pgplot/}}. You can unpack it with the @command{tar xf} command. Let's assume the directory you have unpacked it to is @file{PGPLOT}, most probably it is: @file{/home/username/Downloads/pgplot/}. open the @file{drivers.list} file: @example $ gedit drivers.list @end example @noindent Remove the @code{!} for the following lines and save the file in the end: @example PSDRIV 1 /PS PSDRIV 2 /VPS PSDRIV 3 /CPS PSDRIV 4 /VCPS XWDRIV 1 /XWINDOW XWDRIV 2 /XSERVE @end example @noindent Don't choose GIF or VGIF, there is a problem in their codes. Open the @file{PGPLOT/sys_linux/g77_gcc.conf} file: @example $ gedit PGPLOT/sys_linux/g77_gcc.conf @end example @noindent change the line saying: @code{FCOMPL="g77"} to @code{FCOMPL="gfortran"}, and save it. This is a very important step during the compilation of the code if you are in GNU/Linux. You now have to create a folder in @file{/usr/local}, don't forget to replace @file{PGPLOT} with your unpacked address: @example $ su # mkdir /usr/local/pgplot # cd /usr/local/pgplot # cp PGPLOT/drivers.list ./ @end example To make the Makefile, type the following command: @example # PGPLOT/makemake PGPLOT linux g77_gcc @end example @noindent It should finish by saying: @command{Determining object file dependencies}. You have done the hard part! The rest is easy: run these three commands in order: @example # make # make clean # make cpg @end example Finally you have to place the position of this directory you just made into the @command{LD_LIBRARY_PATH} environment variable and define the environment variable @command{PGPLOT_DIR}. To do that, you have to edit your @file{.bashrc} file: @example $ cd ~ $ gedit .bashrc @end example @noindent Copy these lines into the text editor and save it: @cindex @file{LD_LIBRARY_PATH} @example PGPLOT_DIR="/usr/local/pgplot/"; export PGPLOT_DIR LD_LIBRARY_PATH=$LD_LIBRARY_PATH:/usr/local/pgplot/ export LD_LIBRARY_PATH @end example @noindent You need to log out and log back in again so these definitions take effect. After you logged back in, you want to see the result of all this labor, right? Tim Pearson has done that for you, create a temporary folder in your home directory and copy all the demonstration files in it: @example $ cd ~ $ mkdir temp $ cd temp $ cp /usr/local/pgplot/pgdemo* ./ $ ls @end example You will see a lot of pgdemoXX files, where XX is a number. In order to execute them type the following command and drink your coffee while looking at all the beautiful plots! You are now ready to create your own. @example $ ./pgdemoXX @end example @node GNU Free Doc. License, Index, Other useful software, Top @appendix GNU Free Doc. License @cindex GNU Free Documentation License @include fdl.texi @c Print the index and finish: @node Index, , GNU Free Doc. License, Top @unnumbered Index: Macros, structures and functions All Gnuastro library's exported macros start with @code{GAL_}, and its exported structures and functions start with @code{gal_}. This abbreviation stands for @emph{G}NU @emph{A}stronomy @emph{L}ibrary. The next element in the name is the name of the header which declares or defines them, so to use the @code{gal_array_fset_const} function, you have to @code{#include }. See @ref{Gnuastro library} for more. The @code{pthread_barrier} constructs are our implementation and are only available on systems that don't have them, see @ref{Implementation of pthread_barrier}. @printindex fn @unnumbered Index @printindex cp @bye gnuastro-0.5/doc/README0000644000175000017500000000371412722534072011577 00000000000000Documentation of GNU Astronomy Utilities ======================================== This directory contains the documentation (manual) of GNU Astronomy Utilities (Gnuastro) and also all the files necessary for the Gnuastro webpage. Note that only the basic files needed to make the webpage are version controlled. The generated files are not. Documentation (manual): ----------------------- The documentation of Gnuastro is written in Texinfo. The main source file is `gnuastro.texi'. Webpage (only for maintainer) ----------------------------- The top Gnuastro webpage files are also held here, after all, a webpage is another form of documentation. To update the webpage, run the following script: $ ./forwebpage This script will generate the webpage using Gnulib's gendocs.sh script (which was part of the bootstrapping process), then it will copy them all in a specified directory anywhere you like (specified by the TOPWEBCHECKOUT shell variable). You don't have to version control any of the files in that directory, but it is easiest to have a fixed place since CVS needs a local copy. Unfortunately the GNU webpage runs on CVS! Read the top comments of the `forwebpage' script for instructions on what to do for the first time and later times. Update MathJax (for the webpage, only for maintainer) ----------------------------------------------------- There is a script in the `MathJax' directory on the Gnuastro webpage directory to update MathJax (`addmissing.sh'). You can get a recent version of MathJax from its webpage and put it in the correct place (see the comments in the script). 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= @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ 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$(toputildir)/arithmetic/astarithmetic man/astbuildprog.1: $(top_srcdir)/bin/buildprog/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "compile, link with Gnuastro library and its dependencies, and run a C program" \ --libtool $(toputildir)/buildprog/astbuildprog man/astconvertt.1: $(top_srcdir)/bin/convertt/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "convert known data types to each other" \ --libtool $(toputildir)/convertt/astconvertt man/astconvolve.1: $(top_srcdir)/bin/convolve/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "convolve an image with a given kernel" \ --libtool $(toputildir)/convolve/astconvolve man/astcosmiccal.1: $(top_srcdir)/bin/cosmiccal/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "estimate cosmological values" \ --libtool $(toputildir)/cosmiccal/astcosmiccal man/astcrop.1: $(top_srcdir)/bin/crop/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "crop regions of a dataset" \ --libtool $(toputildir)/crop/astcrop man/astfits.1: $(top_srcdir)/bin/fits/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "view and manipulate FITS headers" \ --libtool $(toputildir)/fits/astfits man/astmatch.1: $(top_srcdir)/bin/match/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "match catalogs by 1D or 2D positions" \ --libtool $(toputildir)/match/astmatch man/astmkcatalog.1: $(top_srcdir)/bin/mkcatalog/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "Make a catalog from labeled input images" \ --libtool $(toputildir)/mkcatalog/astmkcatalog man/astmknoise.1: $(top_srcdir)/bin/mknoise/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "add noise to an image" \ --libtool $(toputildir)/mknoise/astmknoise man/astmkprof.1: $(top_srcdir)/bin/mkprof/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "make standard 2D profiles on an image" \ --libtool $(toputildir)/mkprof/astmkprof man/astnoisechisel.1: $(top_srcdir)/bin/noisechisel/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "detect signal in a noisy image" \ --libtool $(toputildir)/noisechisel/astnoisechisel man/aststatistics.1: $(top_srcdir)/bin/statistics/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "calculate statistics of a dataset" \ --libtool $(toputildir)/statistics/aststatistics man/asttable.1: $(top_srcdir)/bin/table/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "read and write ASCII and FITS tables" \ --libtool $(toputildir)/table/asttable #man/astTEMPLATE.1: $(top_srcdir)/bin/TEMPLATE/args.h $(ALLMANSDEP) # $(MAYBE_HELP2MAN) -n "put a short description here" \ # $(toputildir)/TEMPLATE/astTEMPLATE man/astwarp.1: $(top_srcdir)/bin/warp/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "warp (transform) input dataset" \ --libtool $(toputildir)/warp/astwarp # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.5/doc/authors.texi0000644000175000017500000000034413217220432013263 00000000000000Mohammad Akhlaghi (mohammad@@akhlaghi.org, 883)@* Mos@`e Giordano (mose@@gnu.org, 29)@* Vladimir Markelov (vmatroskin@@gmail.com, 18)@* Boud Roukema (boud@@cosmo.torun.pl, 7)@* Lucas MacQuarrie (macquarrielucas@@gmail.com, 1)@* gnuastro-0.5/doc/formath.texi0000644000175000017500000000262212460442046013245 00000000000000@ignore Some macros to be able to show math nicely in HTML and TeX. The problem is that when you use braces in the TeX commands, Texinfo will complain for other formats and when you quote the braces with the at sign, e.g. @{, then TeX will not see the brace properly. So I made two macro functions: mymath{} and dispmath{}. The first is for inline math and the second is for display math where the equation has a line of its own. For the other formats, everything is normal, except the display math equations that don't have any proper solution, so I have just put a $$ $$ around the math. Copying and distribution of this file, with or without modification, are permitted in any medium without royalty provided the copyright notice and this notice are preserved. This file is offered as-is, without any warranty. @end ignore @c HTML: @ifhtml @macro mymath{arg} @inlineraw{html,\\(\arg\\\)} @end macro @macro dispmath{arg} @inlineraw{html,$$\arg\$$} @end macro @end ifhtml @c Docbook @ifdocbook @macro mymath{arg} @math{\arg\} @end macro @macro dispmath{arg} @center@inlineraw{docbook,$$\arg\$$} @end macro @end ifdocbook @c info and plaintext @ifinfo @macro mymath{arg} @inlineraw{info,$\arg\$} @end macro @macro dispmath{arg} @center@inlineraw{info,$$\arg\$$} @end macro @end ifinfo @c TeX @iftex @macro mymath{arg} @math{\arg\} @end macro @macro dispmath{arg} @tex $$\arg\$$ @end tex @end macro @end iftex gnuastro-0.5/doc/stamp-vti0000644000175000017500000000014113217220432012545 00000000000000@set UPDATED 22 December 2017 @set UPDATED-MONTH December 2017 @set EDITION 0.5 @set VERSION 0.5 gnuastro-0.5/doc/version.texi0000644000175000017500000000014113217220432013256 00000000000000@set UPDATED 22 December 2017 @set UPDATED-MONTH December 2017 @set EDITION 0.5 @set VERSION 0.5 gnuastro-0.5/doc/Makefile.am0000644000175000017500000001763513215601241012751 00000000000000## Process this file with automake to produce Makefile.inx ## ## This is part of GNU Astronomy Utilities (gnuastro). It will be ## called by the Makefile.am in the top directory. ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## GNU Astronomy Utilities is free software: you can redistribute it ## and/or modify it under the terms of the GNU General Public License ## as published by the Free Software Foundation, either version 3 of ## the License, or (at your option) any later version. ## ## GNU Astronomy Utilities is distributed in the hope that it will be ## useful, but WITHOUT ANY WARRANTY; without even the implied warranty ## of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the ## GNU General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with GNU Astronomy Utilities. If not, see ## . ## Set the shell SHELL=/bin/bash BUILT_SOURCES = $(srcdir)/authors.texi ## fdl.texi (The GNU Free documentation license in Texinfo format) is ## bootstrapped from Gnulib. Therefore it is not in this ## directory. However, it is needed by gnuastro.texi to build the ## documentation. It is the job of AM_MAKEINFOFLAGS, to pass options to the ## documentation build programs. BOOTSTRPDOC is defined in `configure.ac'. bootstrpdoc = $(top_srcdir)/bootstrapped/doc AM_MAKEINFOFLAGS = -I $(bootstrpdoc) -I $(srcdir) # This is just a temporary work-around since Automake does not pass the # AM_MAKEINFOFLAGS to texi2dvi (which builds DVI and PDF outputs). This was # reported in Automake's bug 23599. Note that a space is necessary between # the `-I' and directory for texi2dvi. TEXI2DVI = texi2dvi -I $(bootstrpdoc) -I $(srcdir) ## Commands to make the texinfo tools. info_TEXINFOS = gnuastro.texi gnuastro_TEXINFOS = $(bootstrpdoc)/fdl.texi formath.texi \ $(srcdir)/authors.texi ## Files not predefined by Automake, and not in dependencies that must ## be included in the final tar-ball distribution. EXTRA_DIST = genauthors README ## We want to build the authors.texi file only when we are building in the ## version controlled source. For the non version controlled souce, ## deleting this file is like somehow deleting formath.texi, it will not be ## rebuilt and result in an error. $(srcdir)/authors.texi: $(top_srcdir)/configure $(top_srcdir)/doc/genauthors $(top_srcdir) ## Images: infognuastrodir=$(infodir)/gnuastro-figures/ dist_infognuastro_DATA = $(top_srcdir)/doc/gnuastro-figures/* ## Man pages to build ## ================== ## ## Installing all the programs is not mandatory in Gnuastro. If a program ## is not built, we shouldn't build its man-page either. if COND_ARITHMETIC MAYBE_ARITHMETIC_MAN = man/astarithmetic.1 endif if COND_BUILDPROG MAYBE_BUILDPROG_MAN = man/astbuildprog.1 endif if COND_CONVERTT MAYBE_CONVERTT_MAN = man/astconvertt.1 endif if COND_CONVOLVE MAYBE_CONVOLVE_MAN = man/astconvolve.1 endif if COND_COSMICCAL MAYBE_COSMICCAL_MAN = man/astcosmiccal.1 endif if COND_CROP MAYBE_CROP_MAN = man/astcrop.1 endif if COND_FITS MAYBE_FITS_MAN = man/astfits.1 endif if COND_MATCH MAYBE_MATCH_MAN = man/astmatch.1 endif if COND_MKCATALOG MAYBE_MKCATALOG_MAN = man/astmkcatalog.1 endif if COND_MKNOISE MAYBE_MKNOISE_MAN = man/astmknoise.1 endif if COND_MKPROF MAYBE_MKPROF_MAN = man/astmkprof.1 endif if COND_NOISECHISEL MAYBE_NOISECHISEL_MAN = man/astnoisechisel.1 endif if COND_STATISTICS MAYBE_STATISTICS_MAN = man/aststatistics.1 endif if COND_TABLE MAYBE_TABLE_MAN = man/asttable.1 endif if COND_WARP MAYBE_WARP_MAN = man/astwarp.1 endif #if COND_TEMPLATE # MAYBE_TEMPLATE_MAN = man/astTEMPLATE.1 #endif dist_man_MANS = $(MAYBE_ARITHMETIC_MAN) $(MAYBE_BUILDPROG_MAN) \ $(MAYBE_CONVERTT_MAN) $(MAYBE_CONVOLVE_MAN) $(MAYBE_COSMICCAL_MAN) \ $(MAYBE_CROP_MAN) $(MAYBE_FITS_MAN) $(MAYBE_MATCH_MAN) $(MAYBE_WARP_MAN) \ $(MAYBE_MKCATALOG_MAN) $(MAYBE_MKNOISE_MAN) $(MAYBE_MKPROF_MAN) \ $(MAYBE_NOISECHISEL_MAN) $(MAYBE_STATISTICS_MAN) $(MAYBE_TABLE_MAN) ## See if help2man is present or not. When help2man doesn't exist, we don't ## want to overwhelm the user with any commands, so we just let them know ## that the distributed man pages will be used. if COND_HASHELP2MAN MAYBE_HELP2MAN = help2man --output=$@ --source="$(PACKAGE_STRING)" else MAYBE_HELP2MAN = @echo "Using distributed man page for" endif # Build the `man' directory and then put all the man pages in # it. Unfortunately as far as I know, pattern rules are not portable in all # implementations of Make, so we have to list all the utilities manually. toputildir=$(top_builddir)/bin ALLMANSDEP = $(top_srcdir)/lib/gnuastro-internal/options.h man/astarithmetic.1: $(top_srcdir)/bin/arithmetic/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "arithmetic operations on images and numbers" \ --libtool $(toputildir)/arithmetic/astarithmetic man/astbuildprog.1: $(top_srcdir)/bin/buildprog/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "compile, link with Gnuastro library and its dependencies, and run a C program" \ --libtool $(toputildir)/buildprog/astbuildprog man/astconvertt.1: $(top_srcdir)/bin/convertt/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "convert known data types to each other" \ --libtool $(toputildir)/convertt/astconvertt man/astconvolve.1: $(top_srcdir)/bin/convolve/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "convolve an image with a given kernel" \ --libtool $(toputildir)/convolve/astconvolve man/astcosmiccal.1: $(top_srcdir)/bin/cosmiccal/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "estimate cosmological values" \ --libtool $(toputildir)/cosmiccal/astcosmiccal man/astcrop.1: $(top_srcdir)/bin/crop/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "crop regions of a dataset" \ --libtool $(toputildir)/crop/astcrop man/astfits.1: $(top_srcdir)/bin/fits/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "view and manipulate FITS headers" \ --libtool $(toputildir)/fits/astfits man/astmatch.1: $(top_srcdir)/bin/match/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "match catalogs by 1D or 2D positions" \ --libtool $(toputildir)/match/astmatch man/astmkcatalog.1: $(top_srcdir)/bin/mkcatalog/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "Make a catalog from labeled input images" \ --libtool $(toputildir)/mkcatalog/astmkcatalog man/astmknoise.1: $(top_srcdir)/bin/mknoise/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "add noise to an image" \ --libtool $(toputildir)/mknoise/astmknoise man/astmkprof.1: $(top_srcdir)/bin/mkprof/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "make standard 2D profiles on an image" \ --libtool $(toputildir)/mkprof/astmkprof man/astnoisechisel.1: $(top_srcdir)/bin/noisechisel/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "detect signal in a noisy image" \ --libtool $(toputildir)/noisechisel/astnoisechisel man/aststatistics.1: $(top_srcdir)/bin/statistics/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "calculate statistics of a dataset" \ --libtool $(toputildir)/statistics/aststatistics man/asttable.1: $(top_srcdir)/bin/table/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "read and write ASCII and FITS tables" \ --libtool $(toputildir)/table/asttable #man/astTEMPLATE.1: $(top_srcdir)/bin/TEMPLATE/args.h $(ALLMANSDEP) # $(MAYBE_HELP2MAN) -n "put a short description here" \ $(toputildir)/TEMPLATE/astTEMPLATE man/astwarp.1: $(top_srcdir)/bin/warp/args.h $(ALLMANSDEP) $(MAYBE_HELP2MAN) -n "warp (transform) input dataset" \ --libtool $(toputildir)/warp/astwarp gnuastro-0.5/doc/man/0000755000175000017500000000000013217220467011545 500000000000000gnuastro-0.5/doc/man/asttable.10000644000175000017500000000777313217220432013354 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH TABLE "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Table \- read and write ASCII and FITS tables .SH SYNOPSIS .B asttable [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Table is part of GNU Astronomy Utilities 0.5. Table can be used to view the information, select columns, or convert tables. The inputs and outputs can be plain text (with white\-space or comma as delimiters), FITS ascii, or FITS binary tables. The output columns can either be selected by number (counting from 1), name or using regular expressions. For regular expressions, enclose the value to the `\-\-column' (`\-c') option in slashes (`\e', as in `\-c\e^mag\e'). To print the selected columns on the command\-line, don't specify an output file. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Table's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ asttable \fB\-P\fR .TP Inputs/Outputs and options: $ info asttable .TP Full section in manual/book: $ info Table .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Table options: .IP Input: .TP \fB\-c\fR, \fB\-\-column\fR=\fI\,STR\/\fR Column number (counting from 1) or search string. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .TP \fB\-\-searchin\fR=\fI\,STR\/\fR Select column(s) in: `name', `unit', `comment'. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-\-tableformat\fR=\fI\,STR\/\fR Table format: `fits\-ascii', `fits\-binary'. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR Type of output: e.g., int16, float32, etc... .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-i\fR, \fB\-\-information\fR Only print table and column information. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Table is maintained as a Texinfo manual. If the .B info and .B Table programs are properly installed at your site, the command .IP .B info Table .PP should give you access to the complete manual. gnuastro-0.5/doc/man/aststatistics.10000644000175000017500000001641313217220432014446 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH STATISTICS "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Statistics \- calculate statistics of a dataset .SH SYNOPSIS .B aststatistics [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Statistics is part of GNU Astronomy Utilities 0.5. Statistics will do statistical analysis on the input dataset (table column or image). All blank pixels or pixels outside of the given range are ignored. You can either directly ask for certain statistics in one line/row as shown below with the same order as requested, or get tables of different statistical measures like the histogram, cumulative frequency style and etc. If no particular statistic is requested, some basic information about the dataset is printed on the command\-line. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Statistics's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ aststatistics \fB\-P\fR .TP Inputs/Outputs and options: $ info aststatistics .TP Full section in manual/book: $ info Statistics .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Statistics options: .IP Input: .TP \fB\-c\fR, \fB\-\-column\fR=\fI\,STR\/\fR Column name or number if input is a table. .TP \fB\-g\fR, \fB\-\-greaterequal\fR=\fI\,FLT\/\fR Only use values greater\-equal than this. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .TP \fB\-l\fR, \fB\-\-lessthan\fR=\fI\,FLT\/\fR Only use values less than this. .TP \fB\-Q\fR, \fB\-\-qrange\fR=\fI\,FLT[\/\fR,FLT] Quantile range: one (from Q to 1\-Q) or two. .TP \fB\-r\fR, \fB\-\-refcol\fR=\fI\,STR\/\fR Reference column name or number. .TP \fB\-\-searchin\fR=\fI\,STR\/\fR Select column(s) in: `name', `unit', `comment'. .IP Tessellation (tile grid): .TP \fB\-\-checktiles\fR Tile IDs in an image, the size of input. .TP \fB\-F\fR, \fB\-\-remainderfrac\fR=\fI\,FLT\/\fR Fraction of remainder to split last tile. .TP \fB\-i\fR, \fB\-\-interpolate\fR Interpolate over blank tiles to fill them. .TP \fB\-\-interpnumngb\fR=\fI\,INT\/\fR No. of neighbors to use for interpolation. .TP \fB\-\-interponlyblank\fR Only interpolate over the blank tiles. .HP \fB\-M\fR, \fB\-\-numchannels\fR=\fI\,INT[\/\fR,..] No. of channels in dim.s (FITS order). .TP \fB\-\-oneelempertile\fR Display 1 element/tile, not full input res. .TP \fB\-\-workoverch\fR Work (not tile) over channel edges. .TP \fB\-Z\fR, \fB\-\-tilesize\fR=\fI\,INT[\/\fR,INT] Regular tile size on dim.s (FITS order). .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-\-tableformat\fR=\fI\,STR\/\fR Table format: `fits\-ascii', `fits\-binary'. .IP Single value measurements .TP \fB\-d\fR, \fB\-\-std\fR Standad deviation. .TP \fB\-E\fR, \fB\-\-median\fR Median. .TP \fB\-\-maximum\fR Maximum. .TP \fB\-\-minimum\fR Minimum. .TP \fB\-m\fR, \fB\-\-mean\fR Mean. .TP \fB\-\-modequant\fR Mode quantile (see \fB\-\-mode\fR) .TP \fB\-\-modesym\fR Mode symmetricity (see \fB\-\-mode\fR). .TP \fB\-\-modesymvalue\fR Value at mode symmetricity (see \fB\-\-mode\fR). .TP \fB\-\-number\fR Number (non\-blank). .TP \fB\-O\fR, \fB\-\-mode\fR Mode (Appendix C of arXiv:1505.01664). .TP \fB\-\-quantfunc\fR=\fI\,FLT[\/\fR,...] Quantile function (multiple values acceptable). .TP \fB\-\-sum\fR Sum. .TP \fB\-u\fR, \fB\-\-quantile\fR=\fI\,FLT[\/\fR,...] Quantile (multiple values acceptable). .IP Particular calculation .TP \fB\-\-asciicfp\fR Print an ASCII cumulative frequency plot. .TP \fB\-A\fR, \fB\-\-asciihist\fR Print an ASCII histogram. .TP \fB\-C\fR, \fB\-\-cumulative\fR Save the cumulative frequency plot in output. .TP \fB\-H\fR, \fB\-\-histogram\fR Save the histogram in output. .TP \fB\-\-mirror\fR=\fI\,FLT\/\fR Save the histogram and CFP of the mirror dist. .TP \fB\-s\fR, \fB\-\-sigmaclip\fR Overall sigma\-clipping (see `\-\-sclipparams') .TP \fB\-t\fR, \fB\-\-ontile\fR Single values on separate tiles, not full input. .TP \fB\-y\fR, \fB\-\-sky\fR Find the Sky and its STD over the tessellation. .IP Sky and Sky STD settings .TP \fB\-\-checksky\fR Store steps in `_sky_steps.fits' file. .TP \fB\-k\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR File name of kernel to convolve input. .TP \fB\-\-khdu\fR=\fI\,STR\/\fR HDU/extension name or number of kernel. .TP \fB\-\-mirrordist\fR=\fI\,FLT\/\fR Max. distance (error multip.) to find mode. .TP \fB\-\-modmedqdiff\fR=\fI\,FLT\/\fR Max. mode and median quantile diff. per tile. .TP \fB\-\-sclipparams\fR=\fI\,FLT\/\fR,FLT Sigma clip: Multiple, and tolerance/number. .TP \fB\-\-smoothwidth\fR=\fI\,INT\/\fR Sky: flat kernel width to smooth interpolated. .IP Histogram and CFP settings .TP \fB\-\-asciiheight\fR=\fI\,INT\/\fR Height of ASCII histogram or CFP plots. .TP \fB\-\-maxbinone\fR Scale such that the maximum bin has value of one. .TP \fB\-\-numasciibins\fR=\fI\,INT\/\fR No. of bins in ASCII histogram or CFP plots. .TP \fB\-\-numbins\fR=\fI\,INT\/\fR No. of bins in histogram or CFP tables. .TP \fB\-n\fR, \fB\-\-normalize\fR Set sum of all bins to 1. .TP \fB\-\-onebinstart\fR=\fI\,FLT\/\fR Shift bins so one bin starts on this value. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Statistics is maintained as a Texinfo manual. If the .B info and .B Statistics programs are properly installed at your site, the command .IP .B info Statistics .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astnoisechisel.10000644000175000017500000001656513217220432014571 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH NOISECHISEL "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME NoiseChisel \- detect signal in a noisy image .SH SYNOPSIS .B astnoisechisel [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION NoiseChisel is part of GNU Astronomy Utilities 0.5. NoiseChisel Detects and segments signal that is deeply burried in noise. It employs a noise\-based detection and segmentation method enabling it to be very resilient to the rich diversity of shapes in astronomical targets. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of NoiseChisel's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astnoisechisel \fB\-P\fR .TP Inputs/Outputs and options: $ info astnoisechisel .TP Full section in manual/book: $ info NoiseChisel .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP NoiseChisel options: .IP Input: .TP \fB\-B\fR, \fB\-\-minskyfrac\fR=\fI\,FLT\/\fR Min. fraction of undetected area in tile. .TP \fB\-\-convolved\fR=\fI\,STR\/\fR Convolved image file to avoid convolution. .TP \fB\-\-convolvedhdu\fR=\fI\,STR\/\fR HDU/extension of convolved image in file. .TP \fB\-E\fR, \fB\-\-skysubtracted\fR Input is Sky subtracted (for error estimation). .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-k\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR Filename of kernel to convolve with input .TP \fB\-\-khdu\fR=\fI\,STR\/\fR HDU containing kernel image. .TP \fB\-\-minnumfalse\fR=\fI\,INT\/\fR Minimum number for S/N estimation. .TP \fB\-w\fR, \fB\-\-widekernel\fR=\fI\,STR\/\fR Filename of wider kernel for better qthresh .TP \fB\-\-wkhdu\fR=\fI\,STR\/\fR HDU containing wide kernel image. .IP Tessellation (tile grid): .TP \fB\-\-checktiles\fR Tile IDs in an image, the size of input. .TP \fB\-F\fR, \fB\-\-remainderfrac\fR=\fI\,FLT\/\fR Fraction of remainder to split last tile. .TP \fB\-\-interpnumngb\fR=\fI\,INT\/\fR No. of neighbors to use for interpolation. .TP \fB\-\-interponlyblank\fR Only interpolate over the blank tiles. .TP \fB\-L\fR, \fB\-\-largetilesize\fR=\fI\,INT[\/\fR,INT] Sim. to \fB\-\-tilesize\fR, but for larger tiles. .HP \fB\-M\fR, \fB\-\-numchannels\fR=\fI\,INT[\/\fR,..] No. of channels in dim.s (FITS order). .TP \fB\-\-oneelempertile\fR Display 1 element/tile, not full input res. .TP \fB\-\-workoverch\fR Work (not tile) over channel edges. .TP \fB\-Z\fR, \fB\-\-tilesize\fR=\fI\,INT[\/\fR,INT] Regular tile size on dim.s (FITS order). .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-\-onlydetection\fR Stop at the end of detection. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-\-tableformat\fR=\fI\,STR\/\fR `txt', `fits\-ascii', `fits\-binary'. .IP Detection: .TP \fB\-\-checkdetection\fR Save all the detection steps to a file. .TP \fB\-\-checkdetsky\fR Save Sky value estimation for pseudo\-dets. .TP \fB\-\-checkdetsn\fR Save pseudo\-detection S/N values to a file. .TP \fB\-\-checkqthresh\fR Save quantile threshold estimation in file. .TP \fB\-c\fR, \fB\-\-detquant\fR=\fI\,FLT\/\fR Quantile in pseudo\-det. to define true. .TP \fB\-\-checksky\fR Final sky and its STD steps in a file. .TP \fB\-\-cleangrowndet\fR Remove small S/N grown detections. .TP \fB\-d\fR, \fB\-\-detgrowquant\fR=\fI\,FLT\/\fR Minimum quant. to expand true detections. .TP \fB\-\-detgrowmaxholesize\fR=\fI\,INT\/\fR Max. area of holes after growth to fill. .TP \fB\-e\fR, \fB\-\-erode\fR=\fI\,INT\/\fR Number of erosions after thresholding. .TP \fB\-\-erodengb\fR=\fI\,INT\/\fR 4 or 8 connectivity in erosion. .TP \fB\-i\fR, \fB\-\-detsnminarea\fR=\fI\,INT\/\fR Min. pseudo\-detection area for S/N dist. .TP \fB\-\-noerodequant\fR=\fI\,FLT\/\fR Quantile for no erosion. .TP \fB\-\-openingngb\fR=\fI\,INT\/\fR 4 or 8 connectivity in opening. .TP \fB\-p\fR, \fB\-\-opening\fR=\fI\,INT\/\fR Depth of opening after erosion. .HP \fB\-\-qthreshtilequant\fR=\fI\,FLT\/\fR Remove tiles at higher quantiles. .TP \fB\-Q\fR, \fB\-\-modmedqdiff\fR=\fI\,FLT\/\fR Max. mode and median quant diff. per tile. .TP \fB\-r\fR, \fB\-\-mirrordist\fR=\fI\,FLT\/\fR Max. dist. (error multip.) to find mode. .TP \fB\-R\fR, \fB\-\-dthresh\fR=\fI\,FLT\/\fR Sigma threshold for Pseudo\-detections. .TP \fB\-\-smoothwidth\fR=\fI\,INT\/\fR Flat kernel width to smooth interpolated. .TP \fB\-s\fR, \fB\-\-sigmaclip\fR=\fI\,FLT\/\fR,FLT Sigma multiple and, tolerance or number. .TP \fB\-t\fR, \fB\-\-qthresh\fR=\fI\,FLT\/\fR Quantile threshold on convolved image. .IP Segmentation: .TP \fB\-\-checkclumpsn\fR Save Sky clump S/N values into a file. .TP \fB\-\-checksegmentation\fR Store segmentation steps in a file. .TP \fB\-g\fR, \fB\-\-segquant\fR=\fI\,FLT\/\fR S/N Quantile of true sky clumps. .TP \fB\-\-grownclumps\fR Save grown clumps instead of original. .TP \fB\-G\fR, \fB\-\-gthresh\fR=\fI\,FLT\/\fR Multiple of STD to stop growing clumps. .TP \fB\-m\fR, \fB\-\-segsnminarea\fR=\fI\,INT\/\fR Minimum area of clumps for S/N estimation. .TP \fB\-O\fR, \fB\-\-objbordersn\fR=\fI\,FLT\/\fR Min. S/N for grown clumps as one object. .TP \fB\-v\fR, \fB\-\-keepmaxnearriver\fR Keep clumps with peak touching a river. .TP \fB\-y\fR, \fB\-\-minriverlength\fR=\fI\,INT\/\fR Minimum len of useful grown clump rivers. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-C\fR, \fB\-\-continueaftercheck\fR Continue processing after checks. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B NoiseChisel is maintained as a Texinfo manual. If the .B info and .B NoiseChisel programs are properly installed at your site, the command .IP .B info NoiseChisel .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astmkprof.10000644000175000017500000001504713217220432013554 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH MAKEPROFILES "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME MakeProfiles \- make standard 2D profiles on an image .SH SYNOPSIS .B astmkprof [\fI\,OPTION\/\fR...] [\fI\,Options\/\fR] [\fI\,Catalog\/\fR] .SH DESCRIPTION MakeProfiles is part of GNU Astronomy Utilities 0.5. MakeProfiles will create a FITS image containing any number of mock astronomical profiles based on an input catalog. All the profiles will be built from the center outwards. First by Monte Carlo integration, then using the central pixel position. The tolerance level specifies when the switch will occur. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of MakeProfiles's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astmkprof \fB\-P\fR .TP Inputs/Outputs and options: $ info astmkprof .TP Full section in manual/book: $ info MakeProfiles .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP MakeProfiles options: .IP Input: .TP \fB\-B\fR, \fB\-\-backhdu\fR=\fI\,INT\/\fR/STR HDU of background image. .TP \fB\-C\fR, \fB\-\-clearcanvas\fR All pixels in background image read as zero. .TP \fB\-E\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR Parameters to only build one kernel. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Input catalog HDU name or number (if FITS). .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .TP \fB\-k\fR, \fB\-\-background\fR=\fI\,STR\/\fR A background image to make the profiles on. .TP \fB\-\-searchin\fR=\fI\,STR\/\fR Select column(s) in: `name', `unit', `comment'. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-i\fR, \fB\-\-individual\fR Build all profiles separately. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-m\fR, \fB\-\-nomerged\fR Do not create a merged image of all profiles. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-\-psfinimg\fR PSF profiles made with all in output image. .TP \fB\-s\fR, \fB\-\-oversample\fR=\fI\,INT\/\fR Scale of oversampling (>0 and odd). .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR Type of output: e.g., int16, float32, etc... .TP \fB\-x\fR, \fB\-\-naxis\fR=\fI\,INT[\/\fR,INT,...] Merged image size along each dimension. .IP Profiles: .TP \fB\-c\fR, \fB\-\-prepforconv\fR Shift and expand based on first catalog PSF. .TP \fB\-e\fR, \fB\-\-envseed\fR Use GSL_RNG_SEED environment variable for seed. .TP \fB\-f\fR, \fB\-\-mforflatpix\fR mcol is flat pixel value (when fcol is 5 or 6) .TP \fB\-\-magatpeak\fR Magnitude is for peak pixel, not full profile. .TP \fB\-\-mcolisbrightness\fR mcol is total brightness, not magnitude. .TP \fB\-\-mode\fR=\fI\,STR\/\fR Mode of `\-\-ccol': `img' or `wcs'. .TP \fB\-p\fR, \fB\-\-tunitinp\fR Truncation is in units of pixels, not radius. .TP \fB\-r\fR, \fB\-\-numrandom\fR=\fI\,INT\/\fR No. of random points in Monte Carlo integration. .TP \fB\-R\fR, \fB\-\-replace\fR Replace overlapping profile pixels, don't add. .TP \fB\-t\fR, \fB\-\-tolerance\fR=\fI\,FLT\/\fR Tolerance to switch to less accurate method. .TP \fB\-w\fR, \fB\-\-circumwidth\fR=\fI\,FLT\/\fR Width of circumference (inward) profiles .TP \fB\-X\fR, \fB\-\-shift\fR=\fI\,INT[\/\fR, ...] Shift profile centers in output image. .TP \fB\-z\fR, \fB\-\-zeropoint\fR=\fI\,FLT\/\fR Magnitude zero point. .IP Columns, by info (see `\-\-searchin'), or number (starting from 1): .TP \fB\-\-ccol\fR=\fI\,STR\/\fR/INT Coordinate columns (one call for each dimension). .TP \fB\-\-fcol\fR=\fI\,STR\/\fR/INT sersic (1), moffat (2), gaussian (3), point (4), flat (5), circumference (6), distance (7). .TP \fB\-\-mcol\fR=\fI\,STR\/\fR/INT Magnitude. .TP \fB\-\-ncol\fR=\fI\,STR\/\fR/INT Sersic index or Moffat beta. .TP \fB\-\-pcol\fR=\fI\,STR\/\fR/INT Position angle. .TP \fB\-\-qcol\fR=\fI\,STR\/\fR/INT Axis ratio. .TP \fB\-\-rcol\fR=\fI\,STR\/\fR/INT Effective radius or FWHM in pixels. .TP \fB\-\-tcol\fR=\fI\,STR\/\fR/INT Truncation in units of \fB\-\-rcol\fR, unless \fB\-\-tunitinp\fR. .IP WCS parameters: .TP \fB\-\-cdelt\fR=\fI\,FLT[\/\fR, ...] Resolution in each dimension. .TP \fB\-\-crpix\fR=\fI\,FLT[\/\fR, ...] Pixel coordinates of reference point. .TP \fB\-\-crval\fR=\fI\,FLT[\/\fR, ...] WCS coordinates of reference point. .TP \fB\-\-ctype\fR=\fI\,STR[\/\fR, ... ] One of FITS standard WCS types. .TP \fB\-\-cunit\fR=\fI\,STR[\/\fR, ... ] Units of the WCS coordinates (e.g., `deg'). .TP \fB\-\-pc\fR=\fI\,FLT[\/\fR, ...] WCS rotation matrix (all elements). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B MakeProfiles is maintained as a Texinfo manual. If the .B info and .B MakeProfiles programs are properly installed at your site, the command .IP .B info MakeProfiles .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astmknoise.10000644000175000017500000000737213217220432013725 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH MAKENOISE "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME MakeNoise \- add noise to an image .SH SYNOPSIS .B astmknoise [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION MakeNoise is part of GNU Astronomy Utilities 0.5. MakeNoise will add noise to all the pixels in an input dataset. The noise parameters can be specified with the options below. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of MakeNoise's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astmknoise \fB\-P\fR .TP Inputs/Outputs and options: $ info astmknoise .TP Full section in manual/book: $ info MakeNoise .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP MakeNoise options: .IP Input: .TP \fB\-b\fR, \fB\-\-background\fR=\fI\,FLT\/\fR Fixed background magnitude for whole input. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-i\fR, \fB\-\-instrumental\fR=\fI\,FLT\/\fR Instrument noise level (in pixel value units). .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .TP \fB\-s\fR, \fB\-\-sigma\fR=\fI\,FLT\/\fR Total noise sigma, ignore other options. .TP \fB\-z\fR, \fB\-\-zeropoint\fR=\fI\,FLT\/\fR Zeropoint magnitude of input. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR Type of output: e.g., int16, float32, etc... .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-e\fR, \fB\-\-envseed\fR Use GSL_RNG_SEED environment variable for seed .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B MakeNoise is maintained as a Texinfo manual. If the .B info and .B MakeNoise programs are properly installed at your site, the command .IP .B info MakeNoise .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astmkcatalog.10000644000175000017500000001754713217220432014227 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH MAKECATALOG "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME MakeCatalog \- Make a catalog from labeled input images .SH SYNOPSIS .B astmkcatalog [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION MakeCatalog is part of GNU Astronomy Utilities 0.5. MakeCatalog will create a catalog from an input, labeled, and noise images. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of MakeCatalog's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astmkcatalog \fB\-P\fR .TP Inputs/Outputs and options: $ info astmkcatalog .TP Full section in manual/book: $ info MakeCatalog .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP MakeCatalog options: .IP Input: .TP \fB\-\-clumpshdu\fR=\fI\,STR\/\fR Clump image extension name or number. .TP \fB\-C\fR, \fB\-\-clumpsfile\fR=\fI\,STR\/\fR Image containing clump labels. .TP \fB\-E\fR, \fB\-\-skysubtracted\fR Input is already sky subtracted (for S/N). .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-\-objectshdu\fR=\fI\,STR\/\fR Object image extension name or number. .TP \fB\-O\fR, \fB\-\-objectsfile\fR=\fI\,STR\/\fR Image containing object/detection labels. .TP \fB\-R\fR, \fB\-\-threshold\fR=\fI\,FLT\/\fR Use pixels more than this multiple of STD. .TP \fB\-s\fR, \fB\-\-skyfile\fR=\fI\,STR\/\fR Image containing sky values. .TP \fB\-\-skyhdu\fR=\fI\,STR\/\fR Sky image extension name or number. .TP \fB\-\-stdhdu\fR=\fI\,STR\/\fR Sky image extension name or number. .TP \fB\-t\fR, \fB\-\-stdfile\fR=\fI\,STR\/\fR Image containing sky STD values. .TP \fB\-\-zeropoint\fR=\fI\,FLT\/\fR Zeropoint magnitude of input dataset. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-\-sfmagarea\fR=\fI\,FLT\/\fR Surface brightness area (in arcseconds^2). .TP \fB\-\-sfmagnsigma\fR=\fI\,FLT\/\fR Surface brightness multiple of Sky STD. .TP \fB\-\-tableformat\fR=\fI\,STR\/\fR Table format: `fits\-ascii', `fits\-binary'. .IP Upper limit magnitude settings: .TP \fB\-e\fR, \fB\-\-envseed\fR Use GSL_RNG_SEED environment variable for seed. .TP \fB\-\-upmaskfile\fR=\fI\,STR\/\fR Mask image file name only for upper limit. .TP \fB\-\-upmaskhdu\fR=\fI\,STR\/\fR Mask image HDU only for upper limit. .TP \fB\-\-upnsigma\fR=\fI\,FLT\/\fR Multiple of sigma to define upperlimit. .TP \fB\-\-upnum\fR=\fI\,INT\/\fR Number of randomly positioned samples .TP \fB\-\-uprange\fR=\fI\,INT\/\fR,INT Range of random positions (pix) around target. .TP \fB\-\-upsigmaclip\fR=\fI\,FLT\/\fR,FLT Sigma multiple and, tolerance or number. .IP Identifier columns .TP \fB\-i\fR, \fB\-\-ids\fR All IDs of objects and clumps. .TP \fB\-\-idinhostobj\fR ID of clump in host object. .TP \fB\-j\fR, \fB\-\-hostobjid\fR ID of object hosting this clump. .TP \fB\-\-objid\fR Object label/ID. .IP Positional columns (pixel) .TP \fB\-\-clumpsgeox\fR Geometric center of all clumps in obj. (X). .TP \fB\-\-clumpsgeoy\fR Geometric center of all clumps in obj. (Y). .TP \fB\-\-clumpsx\fR Flux.wht center of all clumps in obj. (X). .TP \fB\-\-clumpsy\fR Flux.wht center of all clumps in obj. (Y). .TP \fB\-\-geox\fR Geometric center in first FITS axis. .TP \fB\-\-geoy\fR Geometric center in second FITS axis. .TP \fB\-x\fR, \fB\-\-x\fR Flux weighted center in first FITS axis. .TP \fB\-y\fR, \fB\-\-y\fR Flux weighted center in second FITS axis. .IP Positional columns (WCS) .TP \fB\-\-clumpsgeow1\fR Geometric center of all clumps in 1st WCS. .TP \fB\-\-clumpsgeow2\fR Geometric center of all clumps in 2nd WCS. .TP \fB\-\-clumpsw1\fR Flux.wht center of all clumps in 1st WCS. .TP \fB\-\-clumpsw2\fR Flux.wht center of all clumps in 2nd WCS. .TP \fB\-d\fR, \fB\-\-dec\fR Flux weighted center declination. .TP \fB\-\-geow1\fR Geometric center in first WCS axis. .TP \fB\-\-geow2\fR Geometric center in second WCS axis. .TP \fB\-r\fR, \fB\-\-ra\fR Flux weighted center right ascension. .TP \fB\-\-w1\fR Flux weighted center in first WCS axis. .TP \fB\-\-w2\fR Flux weighted center in second WCS axis. .IP Brightness/magnitude related columns .TP \fB\-b\fR, \fB\-\-brightness\fR Brightness (sum of pixel values). .TP \fB\-\-clumpbrightness\fR Brightness of clumps in an object. .TP \fB\-\-clumpsmagnitude\fR Magnitude of all clumps in object. .TP \fB\-G\fR, \fB\-\-magnitudeerr\fR Magnitude error of objects or clumps. .TP \fB\-m\fR, \fB\-\-magnitude\fR Total magnitude of objects or clumps. .TP \fB\-\-noriverbrightness\fR Sky (not river) subtracted clump brightness. .TP \fB\-n\fR, \fB\-\-sn\fR Signal to noise ratio of objects or clumps. .TP \fB\-\-riverave\fR Average river value surrounding a clump. .TP \fB\-\-rivernum\fR Number of river pixels around a clump. .TP \fB\-\-sky\fR Average Sky value under this clump or object. .TP \fB\-\-std\fR Average Sky standard deviation. .TP \fB\-\-upperlimit\fR Upper\-limit value, use other options to config. .TP \fB\-u\fR, \fB\-\-upperlimitmag\fR Upper\-limit mag. use other options to config. .IP Morphology/shape related columns .TP \fB\-a\fR, \fB\-\-area\fR Number of pixels in clump or object. .TP \fB\-A\fR, \fB\-\-semimajor\fR Flux weighted semi\-major axis. .TP \fB\-B\fR, \fB\-\-semiminor\fR Flux weighted semi\-minor axis. .TP \fB\-c\fR, \fB\-\-numclumps\fR Number of clumps in this object. .TP \fB\-\-clumpsarea\fR Sum of all clump areas in an object. .TP \fB\-\-geoaxisratio\fR Geometric axis ratio. .TP \fB\-\-geopositionangle\fR Geometric position angle. .TP \fB\-\-geosemimajor\fR Geometric semi\-major axis. .TP \fB\-\-geosemiminor\fR Geometric semi\-minor axis. .TP \fB\-p\fR, \fB\-\-positionangle\fR Flux weighted position angle. .TP \fB\-Q\fR, \fB\-\-axisratio\fR Flux weighted axis ratio. .TP \fB\-\-weightarea\fR Area used for flux weighted positions. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B MakeCatalog is maintained as a Texinfo manual. If the .B info and .B MakeCatalog programs are properly installed at your site, the command .IP .B info MakeCatalog .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astwarp.10000644000175000017500000001060313217220432013220 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH WARP "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Warp \- warp (transform) input dataset .SH SYNOPSIS .B astwarp [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Warp is part of GNU Astronomy Utilities 0.5. Warp will warp/transform the input image using an input coordinate matrix. Currently it accepts any general projective mapping (which includes affine mappings as a subset). .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Warp's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astwarp \fB\-P\fR .TP Inputs/Outputs and options: $ info astwarp .TP Full section in manual/book: $ info Warp .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Warp options: .IP Input: .TP \fB\-\-hendwcs\fR=\fI\,INT\/\fR Header keyword number to end reading WCS. .TP \fB\-\-hstartwcs\fR=\fI\,INT\/\fR Header keyword number to start reading WCS. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .IP Output: .TP \fB\-C\fR, \fB\-\-coveredfrac\fR=\fI\,FLT\/\fR Acceptable fraction of output pixel covered. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-k\fR, \fB\-\-keepwcs\fR Do not apply warp to input's WCS .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR Type of output: e.g., int16, float32, etc... .IP Warps: .TP \fB\-a\fR, \fB\-\-align\fR Align the image and celestial axes. .TP \fB\-c\fR, \fB\-\-centeroncorner\fR Center of coordinates on first pixel corner. .TP \fB\-e\fR, \fB\-\-shear\fR=\fI\,FLT[\/\fR,FLT] Shear along the given axis(es). .TP \fB\-f\fR, \fB\-\-flip\fR=\fI\,INT[\/\fR,INT] Flip along the given axis(es). .TP \fB\-m\fR, \fB\-\-matrix\fR=\fI\,STR\/\fR Raw transformation matrix, highest priority. .TP \fB\-p\fR, \fB\-\-project\fR=\fI\,FLT[\/\fR,FLT] Project along the given axis(es). .TP \fB\-r\fR, \fB\-\-rotate\fR=\fI\,FLT\/\fR Rotate by the given angle in degrees. .TP \fB\-s\fR, \fB\-\-scale\fR=\fI\,FLT[\/\fR,FLT] Scale along the given axis(es). .TP \fB\-t\fR, \fB\-\-translate\fR=\fI\,FLT[\/\fR,FLT] Translate along the given axis(es). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Warp is maintained as a Texinfo manual. If the .B info and .B Warp programs are properly installed at your site, the command .IP .B info Warp .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astmatch.10000644000175000017500000000771513217220432013355 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH MATCH "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Match \- match catalogs by 1D or 2D positions .SH SYNOPSIS .B astmatch [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Match is part of GNU Astronomy Utilities 0.5. Match matches catalogs of objects and (by default) will return the re\-arranged matching inputs. The optional log file will return low\-level information about the match (indexs and distances). .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Match's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astmatch \fB\-P\fR .TP Inputs/Outputs and options: $ info astmatch .TP Full section in manual/book: $ info Match .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Match options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of first input. .TP \fB\-H\fR, \fB\-\-hdu2\fR=\fI\,STR\/\fR/INT Extension name or number of second input. .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .TP \fB\-\-searchin\fR=\fI\,STR\/\fR Select column(s) in: `name', `unit', `comment'. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-l\fR, \fB\-\-logasoutput\fR No rearranging of inputs, output is log file .TP \fB\-\-notmatched\fR Output is rows that don't match. .TP \fB\-\-outcols\fR=\fI\,STR\/\fR Out cols in CSV, `a': first, `b': second input. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-\-tableformat\fR=\fI\,STR\/\fR Table format: `fits\-ascii', `fits\-binary'. .IP Catalog matching .TP \fB\-a\fR, \fB\-\-aperture\fR=\fI\,FLT[\/\fR,FLT[,FLT]] Acceptable aperture for matching. .TP \fB\-c\fR, \fB\-\-ccol1\fR=\fI\,STR[\/\fR,STR] Column name/number of first catalog. .TP \fB\-C\fR, \fB\-\-ccol2\fR=\fI\,STR[\/\fR,STR] Column name/number of second catalog. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Match is maintained as a Texinfo manual. If the .B info and .B Match programs are properly installed at your site, the command .IP .B info Match .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astfits.10000644000175000017500000000774413217220432013230 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH FITS "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Fits \- view and manipulate FITS headers .SH SYNOPSIS .B astfits [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Fits is part of GNU Astronomy Utilities 0.5. Fits allows you to view and manipulate (add, delete, or modify) FITS extensions (or HDUs) and FITS header keywords within one extension. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Fits's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astfits \fB\-P\fR .TP Inputs/Outputs and options: $ info astfits .TP Full section in manual/book: $ info Fits .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Fits options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .IP Output: .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output file name (only for writing HDUs). .IP HDUs (extensions): .TP \fB\-C\fR, \fB\-\-copy\fR=\fI\,STR\/\fR Copy extension to output file. .TP \fB\-k\fR, \fB\-\-cut\fR=\fI\,STR\/\fR Copy extension to output and remove from input. .TP \fB\-R\fR, \fB\-\-remove\fR=\fI\,STR\/\fR Remove extension from input file. .IP Keywords (in one HDU): .TP \fB\-a\fR, \fB\-\-asis\fR=\fI\,STR\/\fR Write the argument string as is into the header. .TP \fB\-c\fR, \fB\-\-comment\fR=\fI\,STR\/\fR Add COMMENT keyword, any length is ok. .TP \fB\-d\fR, \fB\-\-delete\fR=\fI\,STR\/\fR Delete a keyword from the header. .TP \fB\-H\fR, \fB\-\-history\fR=\fI\,STR\/\fR Add HISTORY keyword, any length is ok. .TP \fB\-p\fR, \fB\-\-printallkeys\fR Print all keywords in the selected HDU. .TP \fB\-r\fR, \fB\-\-rename\fR=\fI\,STR\/\fR Rename keyword, keeping value and comments. .TP \fB\-t\fR, \fB\-\-date\fR Set the DATE keyword to the current time. .TP \fB\-u\fR, \fB\-\-update\fR=\fI\,STR\/\fR Update a keyword value or comments. .TP \fB\-w\fR, \fB\-\-write\fR=\fI\,STR\/\fR Write a keyword (with value, comments and units). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-Q\fR, \fB\-\-quitonerror\fR Quit if there is an error on any action. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Fits is maintained as a Texinfo manual. If the .B info and .B Fits programs are properly installed at your site, the command .IP .B info Fits .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astcrop.10000644000175000017500000001207213217220432013214 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH CROP "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Crop \- crop regions of a dataset .SH SYNOPSIS .B astcrop [\fI\,OPTION\/\fR...] [\fI\,Crop-identifiers\/\fR] \fI\,ASTRdata \/\fR... .SH DESCRIPTION Crop is part of GNU Astronomy Utilities 0.5. Crop will create cutouts, thumbnails, postage stamps or crops of region(s) from input image(s) using image or celestial coordinates. If muliple crops are desired, a catalog must be provided. When in WCS mode, if the cut out covers more than one input image, all overlapping input images will be stitched in the output. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Crop's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astcrop \fB\-P\fR .TP Inputs/Outputs and options: $ info astcrop .TP Full section in manual/book: $ info Crop .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Crop options: .IP Input: .TP \fB\-\-hendwcs\fR=\fI\,INT\/\fR Header keyword number to stop reading WCS. .TP \fB\-\-hstartwcs\fR=\fI\,INT\/\fR Header keyword number to start reading WCS. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of (all) input(s). .TP \fB\-O\fR, \fB\-\-mode\fR=\fI\,STR\/\fR Coordinate mode `img' or `wcs'. .TP \fB\-z\fR, \fB\-\-zeroisnotblank\fR 0.0 in float or double images are not blank. .IP Output: .TP \fB\-b\fR, \fB\-\-noblank\fR Remove parts of the crop box out of input image. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-p\fR, \fB\-\-suffix\fR=\fI\,STR\/\fR Suffix (postfix) of cropped images. .TP \fB\-\-tableformat\fR=\fI\,STR\/\fR Table format: `fits\-ascii', `fits\-binary'. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR Type of output: e.g., int16, float32, etc... .IP Crop by center .TP \fB\-\-checkcenter\fR=\fI\,INT\/\fR Width (in pixels) of box at center to check. .TP \fB\-c\fR, \fB\-\-center\fR=\fI\,FLT[\/\fR,...] Central coordinates of a single crop. .TP \fB\-w\fR, \fB\-\-width\fR=\fI\,FLT[\/\fR,...] Width when crop is defined by its center. .IP Crop by center (when a catalog is given) .TP \fB\-\-cathdu\fR=\fI\,STR\/\fR/INT HDU of catalog, if it is a FITS table. .TP \fB\-C\fR, \fB\-\-catalog\fR=\fI\,STR\/\fR Input catalog filename. .TP \fB\-I\fR, \fB\-\-ignorecase\fR Ignore case in matching/searching columns. .TP \fB\-n\fR, \fB\-\-namecol\fR=\fI\,STR\/\fR/INT Column no./info of crop filename (no suffix). .TP \fB\-\-searchin\fR=\fI\,STR\/\fR Select column(s) in: `name', `unit', `comment'. .TP \fB\-x\fR, \fB\-\-coordcol\fR=\fI\,STR\/\fR/INT Column no./info containing coordinates. .IP Crop by region .TP \fB\-l\fR, \fB\-\-polygon\fR=\fI\,STR\/\fR Polygon vertices of region to crop, keep inside. .TP \fB\-\-outpolygon\fR Keep the polygon's outside, mask the inside. .TP \fB\-s\fR, \fB\-\-section\fR=\fI\,STR\/\fR Image section string specifying crop range. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Crop is maintained as a Texinfo manual. If the .B info and .B Crop programs are properly installed at your site, the command .IP .B info Crop .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astcosmiccal.10000644000175000017500000001013713217220432014206 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH COSMICCALCULATOR "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME CosmicCalculator \- estimate cosmological values .SH SYNOPSIS .B astcosmiccal [\fI\,OPTION\/\fR...] .SH DESCRIPTION CosmicCalculator is part of GNU Astronomy Utilities 0.5. CosmicCalculator will do cosmological calculations. If no redshfit is specified, it will only print the main input parameters. If only a redshift is given, it will print a table of all calculations. If any of the single row calculations are requested, only their values will be printed with a single space between each. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of CosmicCalculator's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astcosmiccal \fB\-P\fR .TP Inputs/Outputs and options: $ info astcosmiccal .TP Full section in manual/book: $ info CosmicCalculator .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP CosmicCalculator options: .IP Input: .TP \fB\-H\fR, \fB\-\-H0\fR=\fI\,FLT\/\fR Current expansion rate (Hubble constant). .TP \fB\-l\fR, \fB\-\-olambda\fR=\fI\,FLT\/\fR Current cosmological cst. dens. per crit. dens. .TP \fB\-m\fR, \fB\-\-omatter\fR=\fI\,FLT\/\fR Current matter density per critical density. .TP \fB\-r\fR, \fB\-\-oradiation\fR=\fI\,FLT\/\fR Current radiation density per critical density. .TP \fB\-z\fR, \fB\-\-redshift\fR=\fI\,FLT\/\fR Redshift of interest. .IP Specific calculations .TP \fB\-a\fR, \fB\-\-absmagconv\fR Conversion to absolute magnitude (no unit). .TP \fB\-A\fR, \fB\-\-angulardimdist\fR Angular diameter distance (Mpc). .TP \fB\-b\fR, \fB\-\-lookbacktime\fR Look back time to z (Gyr). .TP \fB\-c\fR, \fB\-\-criticaldensity\fR Critical density at z (g/cm^3). .TP \fB\-C\fR, \fB\-\-criticaldensitynow\fR Critical density now (g/cm^3). .TP \fB\-d\fR, \fB\-\-properdistance\fR Proper distance to z (Mpc). .TP \fB\-g\fR, \fB\-\-age\fR Age of universe at z (Gyr). .TP \fB\-G\fR, \fB\-\-agenow\fR Age of universe now (Gyr). .TP \fB\-L\fR, \fB\-\-luminositydist\fR Luminosity distance to z (Mpc). .TP \fB\-s\fR, \fB\-\-arcsectandist\fR Tangential dist. covered by 1arcsec at z (kpc). .TP \fB\-u\fR, \fB\-\-distancemodulus\fR Distance modulus at z (no units). .TP \fB\-v\fR, \fB\-\-volume\fR Comoving volume (4pi str) to z (Mpc^3). .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B CosmicCalculator is maintained as a Texinfo manual. If the .B info and .B CosmicCalculator programs are properly installed at your site, the command .IP .B info CosmicCalculator .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astconvolve.10000644000175000017500000001071613217220432014107 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH CONVOLVE "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Convolve \- convolve an image with a given kernel .SH SYNOPSIS .B astconvolve [\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR .SH DESCRIPTION Convolve is part of GNU Astronomy Utilities 0.5. Convolve will convolve an input image with a given spatial kernel (image) in the spatial domain (no edge effects) or frequency domain. The latter suffers from edge effects, but can be much faster. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Convolve's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astconvolve \fB\-P\fR .TP Inputs/Outputs and options: $ info astconvolve .TP Full section in manual/book: $ info Convolve .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Convolve options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Extension name or number of input data. .TP \fB\-H\fR, \fB\-\-minsharpspec\fR=\fI\,FLT\/\fR Deconvolution: min spectrum of sharp img. .TP \fB\-k\fR, \fB\-\-kernel\fR=\fI\,STR\/\fR File name of kernel for convolution. .TP \fB\-\-nokernelflip\fR Do not flip the kernel image. .TP \fB\-\-nokernelnorm\fR Do not normalize the kernel image. .TP \fB\-u\fR, \fB\-\-khdu\fR=\fI\,STR\/\fR HDU containing the kernel. .IP Tessellation (tile grid): .TP \fB\-\-checktiles\fR Tile IDs in an image, the size of input. .TP \fB\-F\fR, \fB\-\-remainderfrac\fR=\fI\,FLT\/\fR Fraction of remainder to split last tile. .HP \fB\-M\fR, \fB\-\-numchannels\fR=\fI\,INT[\/\fR,..] No. of channels in dim.s (FITS order). .TP \fB\-\-oneelempertile\fR Display 1 element/tile, not full input res. .TP \fB\-\-workoverch\fR Work (not tile) over channel edges. .TP \fB\-Z\fR, \fB\-\-tilesize\fR=\fI\,INT[\/\fR,INT] Regular tile size on dim.s (FITS order). .IP Output: .TP \fB\-C\fR, \fB\-\-checkfreqsteps\fR View the steps in the frequency domain. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-\-noedgecorrection\fR Do not correct the edges in the spatial domain .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-T\fR, \fB\-\-type\fR=\fI\,STR\/\fR Type of output: e.g., int16, float32, etc... .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-d\fR, \fB\-\-domain\fR=\fI\,STR\/\fR Convolution domain: `spatial', `frequency'. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-m\fR, \fB\-\-makekernel\fR=\fI\,INT\/\fR Make 2*INT kernel to create input image. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Convolve is maintained as a Texinfo manual. If the .B info and .B Convolve programs are properly installed at your site, the command .IP .B info Convolve .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astconvertt.10000644000175000017500000001040613217220432014114 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH CONVERTTYPE "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME ConvertType \- convert known data types to each other .SH SYNOPSIS .B astconvertt [\fI\,OPTION\/\fR...] \fI\,InputFile1 \/\fR[\fI\,InputFile2\/\fR] ... [\fI\,InputFile4\/\fR] .SH DESCRIPTION ConvertType is part of GNU Astronomy Utilities 0.5. ConvertType will convert any of the known input formats to any other of the known formats. The output file will have the same number of pixels. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of ConvertType's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astconvertt \fB\-P\fR .TP Inputs/Outputs and options: $ info astconvertt .TP Full section in manual/book: $ info ConvertType .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP ConvertType options: .IP Input: .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT FITS input HDU, multiple calls possible. .IP Output: .TP \fB\-b\fR, \fB\-\-borderwidth\fR=\fI\,INT\/\fR EPS/PDF border width in units of 1/72 inch. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output filename or suffix. .TP \fB\-u\fR, \fB\-\-quality\fR=\fI\,INT\/\fR Quality of output JPEG image (1 to 100). .TP \fB\-w\fR, \fB\-\-widthincm\fR=\fI\,FLT\/\fR Width in units of centimeters. .TP \fB\-x\fR, \fB\-\-hex\fR Hexadecimal encoding in EPS. Default: ASCII85. .IP Flux: .TP \fB\-A\fR, \fB\-\-flminbyte\fR Set value of fluxlow as the minimum byte value. .TP \fB\-B\fR, \fB\-\-fhmaxbyte\fR Set value of fluxhigh as the maximum byte value. .TP \fB\-c\fR, \fB\-\-change\fR=\fI\,STR\/\fR Change pixel values `from_1:to_1,from_2:to_2`. .TP \fB\-C\fR, \fB\-\-changeaftertrunc\fR First truncate then change pixel values. .TP \fB\-H\fR, \fB\-\-fluxhigh\fR=\fI\,FLT\/\fR Higher flux truncation value. .TP \fB\-i\fR, \fB\-\-invert\fR Invert the values in JPEG and EPS/PDF. .TP \fB\-L\fR, \fB\-\-fluxlow\fR=\fI\,FLT\/\fR Lower flux truncation value. .TP \fB\-m\fR, \fB\-\-maxbyte\fR=\fI\,INT\/\fR Maximum byte value for all color channels. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B ConvertType is maintained as a Texinfo manual. If the .B info and .B ConvertType programs are properly installed at your site, the command .IP .B info ConvertType .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astbuildprog.10000644000175000017500000001003313217220432014233 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH BUILDPROGRAM "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME BuildProgram \- compile, link with Gnuastro library and its dependencies, and run a C program .SH SYNOPSIS .B astbuildprog [\fI\,OPTION\/\fR...] \fI\,C-source \/\fR[\fI\,ARGUMENTS TO RUN\/\fR] .SH DESCRIPTION BuildProgram is part of GNU Astronomy Utilities 0.5. BuildProgram will compile and run a C program, while automatically linking with libraries that Gnuastro depends on. Hence you do not have to worry about explicitly linking with CFITSIO for example if you want to work on a FITS file, or with GSL if you want to use GNU Scientific Library's functions. The standard compiler options of `\-I', `\-L', and `\-l' are also available for further customization of the build. .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of BuildProgram's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astbuildprog \fB\-P\fR .TP Inputs/Outputs and options: $ info astbuildprog .TP Full section in manual/book: $ info BuildProgram .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP BuildProgram options: .IP Input: .TP \fB\-a\fR, \fB\-\-la\fR=\fI\,STR\/\fR Libtool `.la' to use instead of default. .TP \fB\-I\fR, \fB\-\-includedir\fR=\fI\,STR\/\fR Directories to search for `#include's. .TP \fB\-l\fR, \fB\-\-linklib\fR=\fI\,STR\/\fR Link libraries, e.g., for libgsl: `\-lgsl'. .TP \fB\-L\fR, \fB\-\-linkdir\fR=\fI\,STR\/\fR Directory to search for libraries to link. .TP \fB\-\-tag\fR=\fI\,STR\/\fR Libtool `\-\-tag': programming language. .IP Output: .TP \fB\-b\fR, \fB\-\-onlybuild\fR Don't run the built program. .TP \fB\-\-deletecompiled\fR Delete compiled program after running. .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-g\fR, \fB\-\-debug\fR Debugging information in compiled binary. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .TP \fB\-O\fR, \fB\-\-optimize\fR=\fI\,INT\/\fR Optimization level: 0, 1, 2, 3. .TP \fB\-W\fR, \fB\-\-warning\fR=\fI\,STR\/\fR Compilation warnings on command\-line. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B BuildProgram is maintained as a Texinfo manual. If the .B info and .B BuildProgram programs are properly installed at your site, the command .IP .B info BuildProgram .PP should give you access to the complete manual. gnuastro-0.5/doc/man/astarithmetic.10000644000175000017500000001062713217220432014406 00000000000000.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.5. .TH ARITHMETIC "1" "December 2017" "GNU Astronomy Utilities 0.5" "User Commands" .SH NAME Arithmetic \- arithmetic operations on images and numbers .SH SYNOPSIS .B astarithmetic [\fI\,OPTION\/\fR...] \fI\,ASTRdata or number \/\fR[\fI\,ASTRdata\/\fR] \fI\,OPERATOR \/\fR... .SH DESCRIPTION Arithmetic is part of GNU Astronomy Utilities 0.5. Arithmetic will do arithmetic operations on one or multiple images and numbers. Simply put, the name of the image along with the arithmetic operators and possible numbers are given as arguments. The extensions of each input are specified with (possibly multiple) calls to the `\-\-hdu' option. .PP Currently Arithmetic only supports postfix or reverse polish notation. For example to get the result of `5+6', you should write `5 6 +', or to get the average of two images, you should write `a.fits b.fits + 2 /' (or more simply use the `average' operator with `a.fits b.fits average'). Please see the manual for more information. .PP Arithmetic recognizes a large collection of standard operators, including basic arithmetic (e.g., +, \-, x, /), mathematical (e.g., abs, pow, sqrt, log), statistical (minvalue, min, max, average), comparison (e.g., lt, le, gt), logical (e.g., and, or, not), the full set of bitwise operators, and numeric type conversion operators to all known types. Please run the command below for a complete list describing all operators (press the `SPACE' keyboard key, or arrow keys, to go down and `q' to return to the command\-line): .IP \f(CW$ info gnuastro "Arithmetic operators"\fR .PP For more information, please run any of the following commands. In particular the second contains a very comprehensive explanation of Arithmetic's invocation: expected input(s), output(s), and a full description of all the options. .TP All options and their values: $ astarithmetic \fB\-P\fR .TP Inputs/Outputs and options: $ info astarithmetic .TP Full section in manual/book: $ info Arithmetic .TP Full Gnuastro manual/book: $ info gnuastro .PP If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users and developers. For more information, please run: .IP \f(CW$ info help-gnuastro\fR .PP Arithmetic options: .IP Input: .TP \fB\-g\fR, \fB\-\-globalhdu\fR=\fI\,STR\/\fR Use this HDU for all inputs, ignore `\-\-hdu'. .TP \fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT Nth call, used for HDU of Nth input FITS. .IP Output: .TP \fB\-D\fR, \fB\-\-dontdelete\fR Don't delete output if it exists. .TP \fB\-K\fR, \fB\-\-keepinputdir\fR Keep input directory for automatic output. .TP \fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR Output name. .IP Operating modes: .TP \-?, \fB\-\-help\fR give this help list .TP \fB\-\-cite\fR BibTeX citation for this program. .TP \fB\-\-config\fR=\fI\,STR\/\fR Read configuration file STR immediately. .TP \fB\-\-lastconfig\fR Do not parse any more configuration files. .TP \fB\-\-log\fR Information about output(s) in a log file. .TP \fB\-\-minmapsize\fR=\fI\,INT\/\fR Minimum bytes in array to not use ram RAM. .TP \fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR Number of CPU threads to use. .TP \fB\-\-onlyversion\fR=\fI\,STR\/\fR Only run if the program version is STR. .TP \fB\-P\fR, \fB\-\-printparams\fR Print parameter values to be used and abort. .TP \fB\-q\fR, \fB\-\-quiet\fR Only report errors, remain quiet about steps. .TP \fB\-S\fR, \fB\-\-setdirconf\fR Set default values for this directory and abort. .TP \fB\-\-usage\fR give a short usage message .TP \fB\-U\fR, \fB\-\-setusrconf\fR Set default values for this user and abort. .TP \fB\-V\fR, \fB\-\-version\fR print program version .PP Mandatory or optional arguments to long options are also mandatory or optional for any corresponding short options. .PP GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/ .SH "REPORTING BUGS" Report bugs to bug\-gnuastro@gnu.org. .SH COPYRIGHT Copyright \(co 2015\-2017, Free Software Foundation, Inc. License GPLv3+: GNU General public license version 3 or later. .br This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent permitted by law. .PP Written/developed by Mohammad Akhlaghi .SH "SEE ALSO" The full documentation for .B Arithmetic is maintained as a Texinfo manual. If the .B info and .B Arithmetic programs are properly installed at your site, the command .IP .B info Arithmetic .PP should give you access to the complete manual. gnuastro-0.5/doc/gnuastro-figures/0000755000175000017500000000000013217220467014276 500000000000000gnuastro-0.5/doc/gnuastro-figures/sphereandplane.txt0000644000175000017500000000005013217200076017735 00000000000000../gnuastro-figures//sphereandplane.eps gnuastro-0.5/doc/gnuastro-figures/sphereandplane.png0000644000175000017500000003521013217200076017710 00000000000000‰PNG  IHDRʤk­}bKGDÿ‡Ì¿ pHYs––qFþð xzTXtRaw profile type iccX…—m’d© Eÿ³ /O -Šðþ7àCVwO·Ý3c;+ˆÌz„®îéŸîé|êPIù}VÉ?>õë·¹ÚµŽÚµ×šÇ6VÍöIR¤iÓÜËÈ#wÿÓ™ñ v}ýpç´zþCþÇùKº mÒ¾ùòíꉃe­Ú?ÿ_/êT%BùûóõÍNéReÿñ|÷ïÏáü„ñëŸ?èÏÏÿaèçç‘6ÔÉÌ—«5í0³cè÷Ïÿd~úõÌß?µöò,&ÂûIú›„ÇUጚµ}‡F·ÞRoL"JoË\Æï£üw¦ÓÚþoMÿúùÛôë;úü–%>?Èš±‘‰ oØþyô×qhµåVý]‰DÌå»G¥ˆûßÕÒ÷ÏïæI¬ú9Z›ñ‡f¿ŸXÍÞ÷Öù™WæYÿ>ïc¨öoÈù‰Å?È’übñG¤ò3øÅ#Ã0T.¦Ú+ EKÒ2u“ÛþZÙYôvê,<x7Xó°'ó)yGS}E< Úă‰wÀaÀ0°0°x¸0°ë;$ƒ5Îgo =æ8,:`^¾ü¾ûã5LÃØäåý)ãšÆ0FäRƒ÷ J›ŒËQy±²^p¿`£‹…wÊ;¼.#x\Œ9x[ Ö‚§e m~àbq¾߇ïË÷å;X‹âl ‡†;ãP/ÂB;ÉTap4ª™ÁKv¯ÊCe!Ù«óæjL$Çuad³˜ «or2r}9"è´—þ–7à’Uò£ÚÆ.Ô#rƒwšðNñI/€ããŒ7ß6ÿ»æv†°Ü®çF¶…Âi™úa kçÞ'@HwÇãŽÁ>ú^ ‚wxÚ½§ÜˆÉƒI ÔNÅó £- ÜÇ̃£ 2€ÈÀ«±éqÆ lñƒ4þ8¢TÍÈO„쉬,ºÁžg±“eE8,Yn£Ðàœ¬)+˜Pv×vàŒÈT>íYÙY©1%кy~ .6Õ˜Pë¿‘'U0»ä9VÌ7O8dâî\ `ó?‹æÕ<£^xÆ1Lz6µl“ß Þ¸y¤lìb,X¥äűž- ±8Ò¢lXdh‹…š¬xyæBÝÐņ“¶P´›ºÛLÞû•ß~“A/@°®ì@Á‡gݶ|iöWf×1zÞ_E²O¥¶ò!.‡‰ÈgÂá7ñ¸ÀႾKö.ǺùÚ¦%_Bpï¥,ñ(8ó€T±ŠÝPãÈq_y¥J:Œ+œ_qÙ6nóüè[X(äÄà»|{J™^Ê"Zn¥ÜÉá´PW¥öQªôB锺Z©Î¸ù#ôÊ@× â0˜ö JSJ§ðz7Dz•>wéë@—=!‡RËhtBC ²YìTÆ>…S½j+tEX,âEfÙGy«(Ô ½•A¯aE×-`«hh™Cz™¼œs•¹bç7 ?”ÑLv1NjèžCcÒ˪«,B³T¡£[€F*‹€âxÙm—Í177žì³Êc P|ð­»8ñq÷âø@Z‡*>ú(ÌK+c·H¹xw‰Éµ^.€º×Jh·„ð›ç±£Ä]õC¥ÄžÂ«À<:H²#UàäÐl¿ˆ¦ßʪZ«Ö:F­“Ÿ+j=ÍYÞªpUmÖkóšj‹Ç–Q{?tŽÆíÚÏzÕU“‡0úáŒ@ÉëSsÆÔ×¼U¹“üâ‘v«ªTô8êvêlAólŽœ^í‰-F <¢{*lBñà mÌb£Eú¡ã€DjÝM e«›‰ ¢>jófÕåVÇ …3½ârTêaãsÁ% ¹ÝSÅ38\+5S9 \¾jX©ÁQ"`®6`/ŠoQ½gS@¹“>BT6ßQ¾¥V¥µjÞï™­AÎM£µ=[#e_é‘Z·Ûú™t2­ øyLú3¯mÄ¡845Q‚¿n“kˆEoúDüéÑ6Ko4 mNoÓçkV>I26²ÍÁºÃÌÒžGEY¢qâ¶X®ÕödTm_sŽä·µSk£Z8m0L»(ÒeÓ‹"Á$‰ü”L Yjq+ÊبÙþ(ò‘¡…BE/¥P*\¯{P%줇®‰êÈa§ísu*ü‘RFC )séÒk=¡¬Ý%6¢¤º‡`M$»SÈ}BFå˜ÓeN†¼h_z:Žô ü7ñÞÞxMýu’Ú}¯¤:³R?F2Ž÷Kpåv ð¥•´ÊIJÇyBa+±ý¨ª@ ¡ƒAa@0*—P§Zäa]ƒ€Þ±JcÙϦÊæÊAjWi•eƒ.yŒ¡T*žÆ‚SϘ¾‡Á2&á!yYÇbÙZŒcµmŒ‹ÍÆ€ÄüÈ8x{t¦qÜÔ4®ø¸û (/ Õ .¬Î8üË›âX%¢Õ¸ä à³tIC[úKºué×@[E~U„ß” P催‹f…-¨³Ìëò.5b¶Äâ!erô GPÙì¼ßø©â‹k+â~è1Î6¡VåÊ–ë ˆG“€ÓiÇzú–Kn|±¡ô$˜j^8BÙˆõBû×ÝÒÉdCç®Ä&½s©Àì\?i‚t7¡àº>™lu©MÚ† kq±$±49]áwÝÔ¼ª>1äOU¸ßPCúú× ^&Àt0]ãÒeu.»k¾–b¢Q³øD2LG‡4Mªý<¬Ï~)vµéŽ^t+á–õÎd1±8§dp§AÚføwR–i._©ŸÄpîðécðì@]‡5'bÞOrl}3½íÝÒBóYÖL†|@ÚËÐòW,—@9ôT“¢£NÆnŸ2$½FeÓˆƒÍî67ŽÕžð.›…‚iëj¸~¯0dÐœ9j„¡B†îÙ]´º-‚OhoÏLtŠ´ ôÎ0Y4…Ï@);UE™S€sÅ^´*`Pv^­‰LÚãÁ2Åhf|-DEY›2Û×t_N'x:½Z~ÑŽ‹ì?üâÑ~w;J’®k¥M²ËA°:Šï0}#öërBêÔ¨äÒö˜‹þ ¿Õ6ÄèæÆJ›ò>Üfà£m,†¥÷ÚK—ge»í×ðìCkË  q8-P~”4‚¦’V2_: Q‡–`™@õˆ¤.´ýЭ¾9hè\ýG øhÇçvG?ØËhP¦‹ä°…on±Xrâ(–Ãg‡ø}·Û¦€ÛÌÉ›¶­9‡¡ mq¸-Øþ 7‰8~@DýžqˆÖG,Ž=âp¦ ‹l 1y']gÅ&ö4¿ÜB|.Ú¯œ3p?´<'hbq³A.óæqçºãô7;'Û…».2r{8UÍçsÅ$]øâ$‘6`;=Ø?$R]Ò„\6ñ†Z/}ï=æt ó’×(_8}ô˜‰î{D¡_(ô2„¤X@IÑt¶†{Ï ‘ò’F£9™3­% ³¤X´ò[5È'…2‰ Å¡FnßqÑ”mDúí‘ÈK­Šµ.åIDATxÚí{”$WyØW$¡×ÖJ‘ˆ½r-Ø`[ì âhm¨9Xv²ÂF½6Š³„{bäݯIAkëGObEDëÄt#Ùf,Kñ´Ú%>Æé&a6†È‡i`$›cÛGsµ5zìJ+iuóG×ÌtÏt÷ô£ºêÞªï7gÏΣ·ºûWß½_}÷^¥Á$ÎJº°¨jÒ-ƃH)†!R ‚aˆ”‚`"¥ †H)†!R ‚aˆ”‚`"¥Ð媢òAåU^9I·&;ˆ”BTŽœž!§æ©áRHº=Ùᜤ ‹§ghè†jPOº9ÙAIí«­¨ªžŠáYŽ3£+Ik¶î«ÐåâRåȘ2>DJ¡#ÊUUÀ§® Ÿt{²„Œ)…n8*‡K r¸Ôtts²ƒH)tD7˜T®®€rDÈx‘î«ÐÝ%ãF¤Ã)Á0DJA0 ‘R C¤ÃK"BG”K‘¸Žwj©{‘Rèˆn°T‰o‰’q#R ]Q%êÈUÊØ‘1¥ÐU¢®Ë Ü¤[’5DJ¡#«JRNº%ÙCº¯BÖ” Kí„8‘H)lb]I! 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0000000000000000000000000000000000000000000000000000000000000000 cleartomark {restore}if %%BeginFont: CMMI7 %!PS-AdobeFont-1.0: CMMI7 003.002 %%Title: CMMI7 %Version: 003.002 %%CreationDate: Mon Jul 13 16:17:00 2009 %%Creator: David M. 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Jones %Copyright: Copyright (c) 1997, 2009 American Mathematical Society %Copyright: (), with Reserved Font Name CMR7. % This Font Software is licensed under the SIL Open Font License, Version 1.1. % This license is in the accompanying file OFL.txt, and is also % available with a FAQ at: http://scripts.sil.org/OFL. %%EndComments FontDirectory/CMR7 known{/CMR7 findfont dup/UniqueID known{dup /UniqueID get 5000790 eq exch/FontType get 1 eq and}{pop false}ifelse {save true}{false}ifelse}{false}ifelse 11 dict begin /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0 ]readonly def /FontName /CMR7 def /FontBBox {-27 -250 1122 750 }readonly def /PaintType 0 def /FontInfo 9 dict dup begin /version (003.002) readonly def /Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050\051, with Reserved Font Name CMR7.) readonly def /FullName (CMR7) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def 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Jones %Copyright: Copyright (c) 1997, 2009 American Mathematical Society %Copyright: (), with Reserved Font Name CMR10. % This Font Software is licensed under the SIL Open Font License, Version 1.1. % This license is in the accompanying file OFL.txt, and is also % available with a FAQ at: http://scripts.sil.org/OFL. %%EndComments FontDirectory/CMR10 known{/CMR10 findfont dup/UniqueID known{dup /UniqueID get 5000793 eq exch/FontType get 1 eq and}{pop false}ifelse {save true}{false}ifelse}{false}ifelse 11 dict begin /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0 ]readonly def /FontName /CMR10 def /FontBBox {-40 -250 1009 750 }readonly def /PaintType 0 def /FontInfo 9 dict dup begin /version (003.002) readonly def /Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050\051, with Reserved Font Name CMR10.) readonly def /FullName (CMR10) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def 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14.59727 lineto 374.57356 14.43292 lineto 375.38327 14.32823 lineto 376.19298 14.26422 lineto 377.00269 14.2253 lineto pgfstr restore save 0.19925 pgfw 337.32684 17.00824 moveto 337.32684 14.17339 lineto pgfstr save save [1.0 0.0 0.0 1.0 327.88268 5.93782 ] concat pgfs 0 setgray -596 414 a Fe(\000)p Ff(!)-497 422 y Fd(m)-596 414 y pgfr restore restore restore save 0.19925 pgfw 377.01265 17.00824 moveto 377.01265 14.17339 lineto pgfstr save save [1.0 0.0 0.0 1.0 367.56848 5.93782 ] concat pgfs 0 setgray -596 414 a Fg(+)p Ff(!)-497 422 y Fd(m)-596 414 y pgfr restore restore restore 357.16995 14.17339 moveto pgfstr save save [1.0 0.0 0.0 1.0 355.05284 5.51721 ] concat pgfs 0 setgray -596 414 a Fg(0)-596 414 y pgfr restore restore save [ 0.3985 1.99255 ] 0.0 setdash 331.65758 14.17339 moveto 331.65758 99.21382 lineto pgfstr restore save [ 0.3985 1.99255 ] 0.0 setdash 382.68192 14.17339 moveto 382.68192 99.21382 lineto pgfstr restore save 0.5 setgray 0.3985 pgfw 332.11584 90.7097 moveto 382.22363 90.7097 lineto pgfstr save [-1.0 0.0 0.0 -1.0 332.11584 90.7097 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore save [1.0 0.0 0.0 1.0 382.22363 90.7097 ] concat save 0.31879 pgfw [ ] 0.0 setdash 1 setlinecap 1 setlinejoin -1.19551 1.59401 moveto -1.09587 0.99626 0.0 0.09961 0.29886 0.0 curveto 0.0 -0.09961 -1.09587 -0.99626 -1.19551 -1.59401 curveto pgfstr restore restore restore 357.16995 90.7097 moveto pgfstr save save [1.0 0.0 0.0 1.0 351.53423 97.66507 ] concat pgfs 0 setgray -586 381 a Fb(2)p Fc(\031)p -586 395 75 4 v -574 443 a(P)-596 414 y pgfr restore restore save 1.49442 pgfw 388.3512 14.17339 moveto 388.3512 14.22443 lineto 389.1609 14.26335 lineto 389.97061 14.32738 lineto 390.78033 14.43118 lineto 391.59003 14.59468 lineto 392.39975 14.84209 lineto 393.20946 15.21667 lineto 394.01918 15.7608 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003.002 %%Title: CMR7 %Version: 003.002 %%CreationDate: Mon Jul 13 16:17:00 2009 %%Creator: David M. Jones %Copyright: Copyright (c) 1997, 2009 American Mathematical Society %Copyright: (), with Reserved Font Name CMR7. % This Font Software is licensed under the SIL Open Font License, Version 1.1. % This license is in the accompanying file OFL.txt, and is also % available with a FAQ at: http://scripts.sil.org/OFL. %%EndComments FontDirectory/CMR7 known{/CMR7 findfont dup/UniqueID known{dup /UniqueID get 5000790 eq exch/FontType get 1 eq and}{pop false}ifelse {save true}{false}ifelse}{false}ifelse 11 dict begin /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0 ]readonly def /FontName /CMR7 def /FontBBox {-27 -250 1122 750 }readonly def /PaintType 0 def /FontInfo 9 dict dup begin /version (003.002) readonly def /Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050\051, with Reserved Font Name CMR7.) readonly def /FullName (CMR7) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def 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FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFF end %%PageTrailer %%Trailer %%EOF gnuastro-0.5/lib/0000755000175000017500000000000013217220466010772 500000000000000gnuastro-0.5/lib/gnuastro.pc.in0000644000175000017500000000044412765554423013521 00000000000000prefix=@prefix@ exec_prefix=@exec_prefix@ libdir=@libdir@ includedir=@includedir@ Name: Gnuastro Description: GNU Astronomy Utilities URL: https://www.gnu.org/software/gnuastro/ Version: @VERSION@ Requires.private: wcs cfitsio gsl Cflags: -I${includedir} Libs: -L${libdir} -lgnuastro @LIBS@ gnuastro-0.5/lib/wcs.c0000644000175000017500000006474513216276304011673 00000000000000/********************************************************************* Functions to that only use WCSLIB functionality. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /************************************************************* *********** Read WCS *********** *************************************************************/ /* Read the WCS information from the header. Unfortunately, WCS lib is not thread safe, so it needs a mutex. In case you are not using multiple threads, just pass a NULL pointer as the mutex. After you finish with this WCS, you should free the space with: status = wcsvfree(&nwcs,&wcs); If the WCS structure is not recognized, then this function will return a NULL pointer for the wcsprm structure and a zero for nwcs. It will also report the fact to the user in stderr. =================================== WARNING: wcspih IS NOT THREAD SAFE! =================================== Don't call this function within a thread or use a mutex. */ struct wcsprm * gal_wcs_read_fitsptr(fitsfile *fptr, size_t hstartwcs, size_t hendwcs, int *nwcs) { /* Declaratins: */ int nkeys=0, status=0; struct wcsprm *wcs=NULL; char *fullheader, *to, *from; int relax = WCSHDR_all; /* Macro: use all informal WCS extensions. */ int ctrl = 0; /* Don't report why a keyword wasn't used. */ int nreject = 0; /* Number of keywords rejected for syntax. */ /* CFITSIO function: */ if( fits_hdr2str(fptr, 1, NULL, 0, &fullheader, &nkeys, &status) ) gal_fits_io_error(status, NULL); /* Only consider the header keywords in the current range: */ if(hendwcs>hstartwcs) { /* Mark the last character in the desired region. */ fullheader[hendwcs*(FLEN_CARD-1)]='\0'; /*******************************************************/ /****************************************************** printf("%s\n", fullheader); ******************************************************/ /*******************************************************/ /* Shift all the characters to the start of the string. */ if(hstartwcs) /* hstartwcs!=0 */ { to=fullheader; from=&fullheader[hstartwcs*(FLEN_CARD-1)-1]; while(*from++!='\0') *to++=*from; } nkeys=hendwcs-hstartwcs; /*******************************************************/ /****************************************************** printf("\n\n\n###############\n\n\n\n\n\n"); printf("%s\n", &fullheader[1*(FLEN_CARD-1)]); exit(0); ******************************************************/ /*******************************************************/ } /* WCSlib function to parse the FITS headers. */ status=wcspih(fullheader, nkeys, relax, ctrl, &nreject, nwcs, &wcs); if(status) { fprintf(stderr, "\n##################\n" "WCSLIB Warning: wcspih ERROR %d: %s.\n" "##################\n", status, wcs_errmsg[status]); wcs=NULL; *nwcs=0; } if (fits_free_memory(fullheader, &status) ) gal_fits_io_error(status, "problem in fitsarrayvv.c for freeing " "the memory used to keep all the headers"); /* Set the internal structure: */ if(wcs) { /* CTYPE is a mandatory WCS keyword, so if it hasn't been given (its '\0'), then the headers didn't have a WCS structure. However, WCSLIB still fills in the basic information (for example the dimensionality of the dataset). */ if(wcs->ctype[0][0]=='\0') { wcsfree(wcs); wcs=NULL; *nwcs=0; } else { /* Set the WCS structure. */ status=wcsset(wcs); if(status) { fprintf(stderr, "\n##################\n" "WCSLIB Warning: wcsset ERROR %d: %s.\n" "##################\n", status, wcs_errmsg[status]); wcsfree(wcs); wcs=NULL; *nwcs=0; } else /* A correctly useful WCS is present. When no PC matrix elements were present in the header, the default PC matrix (a unity matrix) is used. In this case WCSLIB doesn't set `altlin' (and gives it a value of 0). In Gnuastro, later on, we might need to know the type of the matrix used, so in such a case, we will set `altlin' to 1. */ if(wcs->altlin==0) wcs->altlin=1; } } /* Return the WCS structure. */ return wcs; } struct wcsprm * gal_wcs_read(char *filename, char *hdu, size_t hstartwcs, size_t hendwcs, int *nwcs) { int status=0; fitsfile *fptr; struct wcsprm *wcs; /* Check HDU for realistic conditions: */ fptr=gal_fits_hdu_open_format(filename, hdu, 0); /* Read the WCS information: */ wcs=gal_wcs_read_fitsptr(fptr, hstartwcs, hendwcs, nwcs); /* Close the FITS file and return. */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); return wcs; } /**************************************************************/ /********** Utilities ************/ /**************************************************************/ /* Copy a given WSC structure into another one. */ struct wcsprm * gal_wcs_copy(struct wcsprm *wcs) { struct wcsprm *out; /* If the input WCS is NULL, return a NULL WCS. */ if(wcs) { /* Allocate the output WCS structure. */ errno=0; out=malloc(sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `out'", __func__, sizeof *out); /* Initialize the allocated WCS structure. The WCSLIB manual says "On the first invokation, and only the first invokation, wcsprm::flag must be set to -1 to initialize memory management"*/ out->flag=-1; wcsini(1, wcs->naxis, out); /* Copy the input WCS to the output WSC structure. */ wcscopy(1, wcs, out); } else out=NULL; /* Return the final output. */ return out; } /* Using the block data structure of the tile, add a WCS structure for it. In many cases, tiles are created for internal processing, so there is no need to keep their WCS. Hence for preformance reasons, when creating the tiles they don't have any WCS structure. When needed, this function can be used to add a WCS structure to the tile by copying the WCS structure of its block and correcting its starting points. If the tile already has a WCS structure, this function won't do anything.*/ void gal_wcs_on_tile(gal_data_t *tile) { size_t i, start_ind, ndim=tile->ndim; gal_data_t *block=gal_tile_block(tile); size_t *coord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "coord"); /* If the tile already has a WCS structure, don't do anything. */ if(tile->wcs) return; else { /* Copy the block's WCS into the tile. */ tile->wcs=gal_wcs_copy(block->wcs); /* Find the coordinates of the tile's starting index. */ start_ind=gal_data_ptr_dist(block->array, tile->array, block->type); gal_dimension_index_to_coord(start_ind, ndim, block->dsize, coord); /* Correct the copied WCS structure. Note that crpix is indexed in the FITS/Fortran order while coord is ordered in C, it also starts counting from 1, not zero. */ for(i=0;iwcs->crpix[i] -= coord[ndim-1-i]; /* printf("start_ind: %zu\n", start_ind); printf("coord: %zu, %zu\n", coord[1]+1, coord[0]+1); printf("CRPIX: %f, %f\n", tile->wcs->crpix[0], tile->wcs->crpix[1]); */ } /* Clean up. */ free(coord); } /* Return the Warping matrix of the given WCS structure. This will be the final matrix irrespective of the type of storage in the WCS structure. Recall that the FITS standard has several methods to store the matrix, which is up to this function to account for and return the final matrix. The output is an allocated DxD matrix where `D' is the number of dimensions. */ double * gal_wcs_warp_matrix(struct wcsprm *wcs) { double *out; size_t i, j, size=wcs->naxis*wcs->naxis; /* Allocate the necessary array. */ errno=0; out=malloc(size*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `out'", __func__, size*sizeof *out); /* Fill in the array. */ if(wcs->altlin & 0x1) /* Has a PCi_j array. */ { for(i=0;inaxis;++i) for(j=0;jnaxis;++j) out[i*wcs->naxis+j] = wcs->cdelt[i] * wcs->pc[i*wcs->naxis+j]; } else if(wcs->altlin & 0x2) /* Has CDi_j array. */ { for(i=0;icd[i]; } else error(EXIT_FAILURE, 0, "%s: currently only PCi_ja and CDi_ja keywords " "are recognized", __func__); /* Return the result */ return out; } /* According to the FITS standard, in the `PCi_j' WCS formalism, the matrix elements m_{ij} are encoded in the `PCi_j' keywords and the scale factors are encoded in the `CDELTi' keywords. There is also another formalism (the `CDi_j' formalism) which merges the two into one matrix. However, WCSLIB's internal operations are apparently done in the `PCi_j' formalism. So its outputs are also all in that format by default. When the input is a `CDi_j', WCSLIB will still read the image into the `PCi_j' formalism and the `CDELTi's are set to 1. This function will decompose the two matrices to give a reasonable `CDELTi' and `PCi_j' in such cases. */ void gal_wcs_decompose_pc_cdelt(struct wcsprm *wcs) { double *ps; size_t i, j; /* The correction is only needed when the PC matrix is filled. */ if(wcs->pc) { /* Get the pixel scale. */ ps=gal_wcs_pixel_scale(wcs); /* The PC matrix and the CDELT elements might both contain scale elements (during processing the scalings might be added only to PC elements for example). So to be safe, we first multiply them into one matrix. */ for(i=0;inaxis;++i) for(j=0;jnaxis;++j) wcs->pc[i*wcs->naxis+j] *= wcs->cdelt[i]; /* Set the CDELTs. */ for(i=0; inaxis; ++i) wcs->cdelt[i] = ps[i]; /* Correct the PCi_js */ for(i=0;inaxis;++i) for(j=0;jnaxis;++j) wcs->pc[i*wcs->naxis+j] /= ps[i]; /* Clean up. */ free(ps); /* According to the `wcslib/wcs.h' header: "In particular, wcsset() resets wcsprm::cdelt to unity if CDi_ja is present (and no PCi_ja).". So apparently, when the input is a `CDi_j', it might expect the `CDELTi' elements to be 1.0. But we have changed that here, so we will correct the `altlin' element of the WCS structure to make sure that WCSLIB only looks into the `PCi_j' and `CDELTi' and makes no assumptioins about `CDELTi'. */ wcs->altlin=1; } } /* The distance (along a great circle) on a sphere between two points is calculated here. Since the pixel sides are usually very small, we won't be using the direct formula: cos(distance)=sin(d1)*sin(d2)+cos(d1)*cos(d2)*cos(r1-r2) We will be using the haversine formula which better considering floating point errors (from Wikipedia:) sin^2(distance)/2=sin^2( (d1-d2)/2 )+cos(d1)*cos(d2)*sin^2( (r1-r2)/2 ) Inputs and outputs are all in degrees. */ double gal_wcs_angular_distance_deg(double r1, double d1, double r2, double d2) { /* Convert degrees to radians. */ double r1r=r1*M_PI/180, d1r=d1*M_PI/180; double r2r=r2*M_PI/180, d2r=d2*M_PI/180; /* To make things easier to read: */ double a=sin( (d1r-d2r)/2 ); double b=sin( (r1r-r2r)/2 ); /* Return the result: */ return 2*asin( sqrt( a*a + cos(d1r)*cos(d2r)*b*b) ) * 180/M_PI; } /* Return the pixel scale of the dataset in units of the WCS. */ double * gal_wcs_pixel_scale(struct wcsprm *wcs) { gsl_vector S; gsl_matrix A, V; int warning_printed; size_t i, j, maxj, n=wcs->naxis; double jvmax, *a, *out, maxrow, minrow; double *v=gal_data_malloc_array(GAL_TYPE_FLOAT64, n*n, __func__, "v"); size_t *permutation=gal_data_malloc_array(GAL_TYPE_SIZE_T, n, __func__, "permutation"); gal_data_t *pixscale=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &n, NULL, 0, -1, NULL, NULL, NULL); /* Write the full WCS rotation matrix into an array, irrespective of what style it was stored in the wcsprm structure (`PCi_j' style or `CDi_j' style). */ a=gal_wcs_warp_matrix(wcs); /* To avoid confusing issues with floating point errors being written in the non-diagonal elements of the FITS header PC or CD matrices, we need to check if the minimum and maximum values in each row are not several orders of magnitude apart. Note that in some cases (for example a spectrum), one axis might be in degrees (value around 1e-5) and the other in angestroms (value around 1e-10). So we can't look at the minimum and maximum of the whole matrix. However, in such cases, people will probably not warp/rotate the image to mix the coordinates. So the important thing to check is the minimum and maximum (non-zero) values in each row. */ warning_printed=0; for(i=0;imaxrow) maxrow=fabs(a[i*n+j]); } /* Do the check, print warning and make correction. */ if(maxrow!=minrow && maxrow/minrow>1e4 && warning_printed==0) { fprintf(stderr, "\nWARNING: The input WCS matrix (possibly taken " "from the FITS header keywords starting with `CD' or `PC') " "contains values with very different scales (more than " "10^4 different). This is probably due to floating point " "errors. These values might bias the pixel scale (and " "subsequent) calculations.\n\n" "You can see the respective matrix with one of the " "following two commands (depending on how the FITS file " "was written). Recall that if the desired extension/HDU " "isn't the default, you can choose it with the `--hdu' " "(or `-h') option before the `|' sign in these commands." "\n\n" " $ astfits file.fits -p | grep 'PC._.'\n" " $ astfits file.fits -p | grep 'CD._.'\n\n" "You can delete the ones with obvious floating point " "error values using the following command (assuming you " "want to delete `CD1_2' and `CD2_1'). Afterwards, you can " "rerun your original command to remove this warning " "message and possibly correct errors that it might have " "caused.\n\n" " $ astfits file.fits --delete=CD1_2 --delete=CD2_1\n\n" ); warning_printed=1; } } /* Fill in the necessary GSL vector and Matrix structures. */ S.size=n; S.stride=1; S.data=pixscale->array; V.size1=n; V.size2=n; V.tda=n; V.data=v; A.size1=n; A.size2=n; A.tda=n; A.data=a; /* Run GSL's Singular Value Decomposition, using one-sided Jacobi orthogonalization which computes the singular (scale) values to a higher relative accuracy. */ gsl_linalg_SV_decomp_jacobi(&A, &V, &S); /* The raw pixel scale array produced from the singular value decomposition above is ordered based on values, not the input. So when the pixel scales in all the dimensions aren't the same (the units of the dimensions differ), the order of the values in `pixelscale' will not necessarily correspond to the input's dimensions. To correct the order, we can use the `V' matrix to find the original position of the pixel scale values and then use permutation to re-order it correspondingly. The column with the largest (absolute) value will be taken as the one to be used for each row. */ for(i=0;ijvmax) { maxj=j; jvmax=fabs(v[i*n+j]); } /* Use the column with the maximum value for this dimension. */ permutation[i]=maxj; } /* Apply the permutation described above. */ gal_permutation_apply(pixscale, permutation); /* Clean up and return. */ free(a); free(v); free(permutation); out=pixscale->array; pixscale->array=NULL; gal_data_free(pixscale); return out; } /* Report the arcsec^2 area of the pixels in the image based on the WCS information in that image. */ double gal_wcs_pixel_area_arcsec2(struct wcsprm *wcs) { double out; double *pixscale; /* A small sanity check. Later, when higher dimensions are necessary, we can find which ones correlate to RA and Dec and use them to find the pixel area in arcsec^2. */ if(wcs->naxis!=2) return NAN; /* Check if the units of the axis are degrees or not. Currently all FITS images I have worked with use `deg' for degrees. If other alternatives exist, we can add corrections later. */ if( strcmp("deg", wcs->cunit[0]) || strcmp("deg", wcs->cunit[1]) ) return NAN; /* Get the pixel scales along each axis in degrees, then multiply. */ pixscale=gal_wcs_pixel_scale(wcs); /* Clean up and return the result. */ out = pixscale[0] * pixscale[1] * 3600.0f * 3600.0f; free(pixscale); return out; } /**************************************************************/ /********** Array conversion ************/ /**************************************************************/ /* Some sanity checks for the WCS conversion functions. */ static void wcs_convert_sanity_check_alloc(gal_data_t *coords, struct wcsprm *wcs, const char *func, int **stat, double **phi, double **theta, double **world, double **pixcrd, double **imgcrd) { gal_data_t *tmp; size_t ndim=0, firstsize=0, size=coords->size; for(tmp=coords; tmp!=NULL; tmp=tmp->next) { /* Count how many coordinates are given. */ ++ndim; /* Check the type of the input. */ if(tmp->type!=GAL_TYPE_FLOAT64) error(EXIT_FAILURE, 0, "%s: input coordinates must have `float64' " "type", func); /* Make sure it has a single dimension. */ if(tmp->ndim!=1) error(EXIT_FAILURE, 0, "%s: input coordinates for each dimension " "must each be one dimensional. Coordinate dataset %zu of the " "inputs has %zu dimensions", func, ndim, tmp->ndim); /* See if all inputs have the same size. */ if(ndim==1) firstsize=tmp->size; else if(firstsize!=tmp->size) error(EXIT_FAILURE, 0, "%s: all input coordinates must have the " "same number of elements. Coordinate dataset %zu has %zu " "elements while the first coordinate has %zu", func, ndim, tmp->size, firstsize); } /* See if the number of coordinates given corresponds to the dimensions of the WCS structure. */ if(ndim!=wcs->naxis) error(EXIT_FAILURE, 0, "%s: the number of input coordinates (%zu) does " "not match the dimensions of the input WCS structure (%d)", func, ndim, wcs->naxis); /* Allocate all the necessary arrays. */ *phi = gal_data_malloc_array( GAL_TYPE_FLOAT64, size, __func__, "phi"); *stat = gal_data_calloc_array( GAL_TYPE_INT32, size, __func__, "stat"); *theta = gal_data_malloc_array( GAL_TYPE_FLOAT64, size, __func__, "theta"); *world = gal_data_malloc_array( GAL_TYPE_FLOAT64, ndim*size, __func__, "world"); *imgcrd = gal_data_malloc_array( GAL_TYPE_FLOAT64, ndim*size, __func__, "imgcrd"); *pixcrd = gal_data_malloc_array( GAL_TYPE_FLOAT64, ndim*size, __func__, "pixcrd"); } /* In Gnuastro, each column (coordinate for WCS conversion) is treated as a separate array in a `gal_data_t' that are linked through a linked list. But in WCSLIB, the input is a single array (with multiple columns). This function will convert between the two. */ static void wcs_convert_list_to_array(gal_data_t *list, double *array, int *stat, size_t ndim, int listtoarray) { size_t i, d=0; gal_data_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) { /* Put all this coordinate's values into the single array that is input into or output from WCSLIB. */ for(i=0;isize;++i) { if(listtoarray) array[i*ndim+d] = ((double *)(tmp->array))[i]; else ((double *)(tmp->array))[i] = stat[i] ? NAN : array[i*ndim+d]; } /* Increment the dimension. */ ++d; } } /* Prepare the output of the WCS conversion functions. */ static gal_data_t * wcs_convert_prepare_out(gal_data_t *coords, struct wcsprm *wcs, int inplace) { size_t i; gal_data_t *out=NULL; if(inplace) out=coords; else for(i=0;inaxis;++i) gal_list_data_add_alloc(&out, NULL, GAL_TYPE_FLOAT64, 1, &coords->size, NULL, 0, coords->minmapsize, wcs->ctype[i], wcs->cunit[i], NULL); return out; } /* Convert world coordinates to image coordinates given the input WCS structure. The input must be a linked list of data structures of float64 (`double') type. The top element of the linked list must be the first coordinate and etc. If `inplace' is non-zero, then the output will be written into the input's allocated space. */ gal_data_t * gal_wcs_world_to_img(gal_data_t *coords, struct wcsprm *wcs, int inplace) { gal_data_t *out; int status, *stat=NULL, ncoord=coords->size, nelem=wcs->naxis; double *phi=NULL, *theta=NULL, *world=NULL, *pixcrd=NULL, *imgcrd=NULL; /* Some sanity checks. */ wcs_convert_sanity_check_alloc(coords, wcs, __func__, &stat, &phi, &theta, &world, &pixcrd, &imgcrd); /* Write the values from the input list of separate columns into a single array (WCSLIB input). */ wcs_convert_list_to_array(coords, world, stat, wcs->naxis, 1); /* Use WCSLIB's wcsp2s for the conversion. */ status=wcss2p(wcs, ncoord, nelem, world, phi, theta, imgcrd, pixcrd, stat); if(status) error(EXIT_FAILURE, 0, "%s: wcss2p ERROR %d: %s", __func__, status, wcs_errmsg[status]); /* For a sanity check. { size_t i; printf("\n\n%s sanity check:\n", __func__); for(i=0;isize;++i) printf("(%g, %g) --> (%g, %g), [stat: %d]\n", world[i*2], world[i*2+1], pixcrd[i*2], pixcrd[i*2+1], stat[i]); } */ /* Allocate the output arrays if they were not already allocated. */ out=wcs_convert_prepare_out(coords, wcs, inplace); /* Write the output from a single array (WCSLIB output) into the output list of this function. */ wcs_convert_list_to_array(out, pixcrd, stat, wcs->naxis, 0); /* Clean up. */ free(phi); free(stat); free(theta); free(world); free(pixcrd); /* Return the output list of coordinates. */ return out; } /* Similar to `gal_wcs_world_to_img'. */ gal_data_t * gal_wcs_img_to_world(gal_data_t *coords, struct wcsprm *wcs, int inplace) { gal_data_t *out; int status, *stat=NULL, ncoord=coords->size, nelem=wcs->naxis; double *phi=NULL, *theta=NULL, *world=NULL, *pixcrd=NULL, *imgcrd=NULL; /* Some sanity checks. */ wcs_convert_sanity_check_alloc(coords, wcs, __func__, &stat, &phi, &theta, &world, &pixcrd, &imgcrd); /* Write the values from the input list of separate columns into a single array (WCSLIB input). */ wcs_convert_list_to_array(coords, pixcrd, stat, wcs->naxis, 1); /* Use WCSLIB's wcsp2s for the conversion. */ status=wcsp2s(wcs, ncoord, nelem, pixcrd, imgcrd, phi, theta, world, stat); if(status) error(EXIT_FAILURE, 0, "%s: wcsp2s ERROR %d: %s", __func__, status, wcs_errmsg[status]); /* For a sanity check. { size_t i; printf("\n\n%s sanity check:\n", __func__); for(i=0;isize;++i) printf("(%g, %g) --> (%g, %g), [stat: %d]\n", pixcrd[i*2], pixcrd[i*2+1], world[i*2], world[i*2+1], stat[i]); } */ /* Allocate the output arrays if they were not already allocated. */ out=wcs_convert_prepare_out(coords, wcs, inplace); /* Write the output from a single array (WCSLIB output) into the output list of this function. */ wcs_convert_list_to_array(out, world, stat, wcs->naxis, 0); /* Clean up. */ free(phi); free(stat); free(theta); free(world); free(pixcrd); /* Return the output list of coordinates. */ return out; } gnuastro-0.5/lib/type.c0000644000175000017500000004632413121462410012037 00000000000000/********************************************************************* Type -- Type information and basic operations. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include /************************************************************* ************** General info *************** *************************************************************/ size_t gal_type_sizeof(uint8_t type) { /* Allocate space for the array to keep the image. */ switch(type) { case GAL_TYPE_BIT: error(EXIT_FAILURE, 0, "%s: bit types are not currently supported, " "please get in touch with us to implement it", __func__); /* The parenthesis after sizeof is not a function, it is actually a type cast, so we have put a space between size of and the parenthesis to highlight this. In C, `sizeof' is an operator, not a function.*/ case GAL_TYPE_UINT8: return sizeof (uint8_t); case GAL_TYPE_INT8: return sizeof (int8_t); case GAL_TYPE_UINT16: return sizeof (uint16_t); case GAL_TYPE_INT16: return sizeof (int16_t); case GAL_TYPE_UINT32: return sizeof (uint32_t); case GAL_TYPE_INT32: return sizeof (int32_t); case GAL_TYPE_UINT64: return sizeof (uint64_t); case GAL_TYPE_INT64: return sizeof (int64_t); case GAL_TYPE_FLOAT32: if( sizeof (float) != 4 ) error(EXIT_FAILURE, 0, "%s: `float' is not 32 bits on this machine", __func__); return sizeof (float); case GAL_TYPE_FLOAT64: if( sizeof (double) != 8 ) error(EXIT_FAILURE, 0, "%s: `double' is not 64 bits on this machine", __func__); return sizeof (double); case GAL_TYPE_COMPLEX32: if( sizeof (float) != 4 ) error(EXIT_FAILURE, 0, "%s: `float' is not 32 bits on this machine", __func__); return sizeof (gsl_complex_float); case GAL_TYPE_COMPLEX64: if( sizeof (double) != 8 ) error(EXIT_FAILURE, 0, "%s: `double` is not 64 bits on this machine", __func__); return sizeof (gsl_complex); case GAL_TYPE_STRING: return sizeof (char *); default: error(EXIT_FAILURE, 0, "%s: type value of %d not recognized", __func__, type); } error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can find " "the cause of the problem. Control should not have reached the end of " "this function", __func__, PACKAGE_BUGREPORT); return -1; } char * gal_type_name(uint8_t type, int long_name) { switch(type) { case GAL_TYPE_BIT: if(long_name) return "bit"; else return "b"; case GAL_TYPE_UINT8: if(long_name) return "uint8"; else return "u8"; case GAL_TYPE_INT8: if(long_name) return "int8"; else return "i8"; case GAL_TYPE_UINT16: if(long_name) return "uint16"; else return "u16"; case GAL_TYPE_INT16: if(long_name) return "int16"; else return "i16"; case GAL_TYPE_UINT32: if(long_name) return "uint32"; else return "u32"; case GAL_TYPE_INT32: if(long_name) return "int32"; else return "i32"; case GAL_TYPE_UINT64: if(long_name) return "uint64"; else return "u64"; case GAL_TYPE_INT64: if(long_name) return "int64"; else return "i64"; case GAL_TYPE_FLOAT32: if(long_name) return "float32"; else return "f32"; case GAL_TYPE_FLOAT64: if(long_name) return "float64"; else return "f64"; case GAL_TYPE_COMPLEX32: if(long_name) return "complex32"; else return "c32"; case GAL_TYPE_COMPLEX64: if(long_name) return "complex64"; else return "c64"; case GAL_TYPE_STRING: if(long_name) return "string"; else return "str"; case GAL_TYPE_STRLL: if(long_name) return "string linked list"; else return "strll"; default: error(EXIT_FAILURE, 0, "%s: type value of %d not recognized", __func__, type); } /* Any of the cases above should return this function, so if control reaches here, there is a bug. */ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "address the problem. Control should not have reached the end of " "this function", __func__, PACKAGE_BUGREPORT); return NULL; } uint8_t gal_type_from_name(char *str) { if( !strcmp(str, "b") || !strcmp(str, "bit") ) return GAL_TYPE_BIT; else if( !strcmp(str, "u8") || !strcmp(str, "uint8") ) return GAL_TYPE_UINT8; else if( !strcmp(str, "i8") || !strcmp(str, "int8") ) return GAL_TYPE_INT8; else if( !strcmp(str, "u16") || !strcmp(str, "uint16") ) return GAL_TYPE_UINT16; else if( !strcmp(str, "i16") || !strcmp(str, "int16") ) return GAL_TYPE_INT16; else if( !strcmp(str, "u32") || !strcmp(str, "uint32") ) return GAL_TYPE_UINT32; else if( !strcmp(str, "i32") || !strcmp(str, "int32") ) return GAL_TYPE_INT32; else if( !strcmp(str, "u64") || !strcmp(str, "uint64") ) return GAL_TYPE_UINT64; else if( !strcmp(str, "i64") || !strcmp(str, "int64") ) return GAL_TYPE_INT64; else if( !strcmp(str, "f32") || !strcmp(str, "float32") ) return GAL_TYPE_FLOAT32; else if( !strcmp(str, "f64") || !strcmp(str, "float64") ) return GAL_TYPE_FLOAT64; else if( !strcmp(str, "c32") || !strcmp(str, "complex32") ) return GAL_TYPE_COMPLEX32; else if( !strcmp(str, "c64") || !strcmp(str, "complex64") ) return GAL_TYPE_COMPLEX64; else if( !strcmp(str, "str") || !strcmp(str, "string") ) return GAL_TYPE_STRING; else return GAL_TYPE_INVALID; /* Any of the cases above should return this function, so if control reaches here, there is a bug. */ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "address the problem. Control must not have reached the end of this " "function", __func__, PACKAGE_BUGREPORT); return 0; } /* Put the minimum (or maximum for the `gal_data_type_max') value for the type in the space (that must already be allocated before the call to this function) pointed to by in. */ void gal_type_min(uint8_t type, void *in) { switch(type) { case GAL_TYPE_UINT8: *(uint8_t *) in = 0; break; case GAL_TYPE_INT8: *(int8_t *) in = INT8_MIN; break; case GAL_TYPE_UINT16: *(uint16_t *) in = 0; break; case GAL_TYPE_INT16: *(int16_t *) in = INT16_MIN; break; case GAL_TYPE_UINT32: *(uint32_t *) in = 0; break; case GAL_TYPE_INT32: *(int32_t *) in = INT32_MIN; break; case GAL_TYPE_UINT64: *(uint64_t *) in = 0; break; case GAL_TYPE_INT64: *(int64_t *) in = INT64_MIN; break; case GAL_TYPE_FLOAT32: *(float *) in = -FLT_MAX; break; case GAL_TYPE_FLOAT64: *(double *) in = -DBL_MAX; break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } } void gal_type_max(uint8_t type, void *in) { switch(type) { case GAL_TYPE_UINT8: *(uint8_t *) in = UINT8_MAX; break; case GAL_TYPE_INT8: *(int8_t *) in = INT8_MAX; break; case GAL_TYPE_UINT16: *(uint16_t *) in = UINT16_MAX; break; case GAL_TYPE_INT16: *(int16_t *) in = INT16_MAX; break; case GAL_TYPE_UINT32: *(uint32_t *) in = UINT32_MAX; break; case GAL_TYPE_INT32: *(int32_t *) in = INT32_MAX; break; case GAL_TYPE_UINT64: *(uint64_t *) in = UINT64_MAX; break; case GAL_TYPE_INT64: *(int64_t *) in = INT64_MAX; break; case GAL_TYPE_FLOAT32: *(float *) in = FLT_MAX; break; case GAL_TYPE_FLOAT64: *(double *) in = DBL_MAX; break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } } /* Since linked lists need a different process than arrays, for functions that work on both, it is convenient to simiplify the check with this function. */ int gal_type_is_list(uint8_t type) { return type==GAL_TYPE_STRLL; } int gal_type_out(int first_type, int second_type) { return first_type > second_type ? first_type : second_type; } /************************************************************* ************** To/from string *************** *************************************************************/ /* Write the bit (0 or 1) contents of `in' into a string ready for printing. `size' is used to determine the number of bytes to print. The output string will be dynamically allocated within this function. This can be useful for easy checking of bit flag values, for example in an expression like below: printf("flag: %s\n", gal_type_bit_string(&flag, sizeof flag) ); */ char * gal_type_bit_string(void *in, size_t size) { size_t i; char *byte=in; char *str=gal_data_malloc_array(GAL_TYPE_UINT8, 8*size+1, __func__, "str"); /* Print the bits into the allocated string. This was inspired from http://stackoverflow.com/questions/111928/is-there-a-printf-converter-to-print-in-binary-format */ for(i=0;iINT8_MIN) { i8=d; ptr=&i8; *type=GAL_TYPE_INT8; } else if(d>INT16_MIN) { i16=d; ptr=&i16; *type=GAL_TYPE_INT16; } else if(d>INT32_MIN) { i32=d; ptr=&i32; *type=GAL_TYPE_INT32; } else { i64=d; ptr=&i64; *type=GAL_TYPE_INT64; } } else { if (d<=UINT8_MAX) { u8=d; ptr=&u8; *type=GAL_TYPE_UINT8; } else if(d<=UINT16_MAX) { u16=d; ptr=&u16; *type=GAL_TYPE_UINT16; } else if(d<=UINT32_MAX) { u32=d; ptr=&u32; *type=GAL_TYPE_UINT32; } else { u64=d; ptr=&u64; *type=GAL_TYPE_UINT64; } } } else { /* The maximum number of decimal digits to store in float or double precision floating point are: float: 23 mantissa bits + 1 hidden bit: log(224)÷log(10) = 7.22 double: 52 mantissa bits + 1 hidden bit: log(253)÷log(10) = 15.95 FLT_DIG (at least 6 in ISO C) keeps the number of digits (not zero before or after) that can be represented by a single precision floating point number. If there are more digits, then we should store the value as a double precision. Note that the number can have non-digit characters that we don't want, like: `.', `e', `E', `,'. */ for(cp=string;*cp!='\0';++cp) if(isdigit(*cp) && *cp!='0' && fnz==-1) fnz=cp-string; /* In the previous loop, we went to the end of the string, so `cp' now points to its `\0'. We just have to iterate backwards! */ for(;cp!=string;--cp) if(isdigit(*cp) && *cp!='0') { lnz=cp-string; break; } /* Calculate the number of decimal digits and decide if it the number should be a float or a double. */ if( lnz-fnz < FLT_DIG || ( dFLT_MIN ) ) { f=d; ptr=&f; *type=GAL_TYPE_FLOAT32; } else { ptr=&d; *type=GAL_TYPE_FLOAT64; } } /* Allocate a one-element dataset, then copy the number into it. */ out=gal_data_malloc_array(*type, 1, __func__, "out"); memcpy(out, ptr, gal_type_sizeof(*type)); return out; } gnuastro-0.5/lib/txt.c0000644000175000017500000012470213211076737011707 00000000000000/********************************************************************* txt -- functions to deal with plain text files. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include /************************************************************************/ /*************** Get table information ***************/ /************************************************************************/ /* Format of table. Currently these constants are internal to this library, we don't want to crowd the name space of the user by having them in the header file. */ enum txt_formats_code { TXT_FORMAT_INVALID, TXT_FORMAT_TABLE, TXT_FORMAT_IMAGE, }; /* Return one of the `txt_line_stat' constant values. */ int gal_txt_line_stat(char *line) { while(*line!='\n') { switch(*line) { /* Characters to ignore. */ case ' ': case ',': case '\t': break; case '#': return GAL_TXT_LINESTAT_COMMENT; default: return GAL_TXT_LINESTAT_DATAROW; } ++line; } return GAL_TXT_LINESTAT_BLANK; } /* Remove the spaces around the values, and if the final/trimmed string has no length, return NULL. */ static char * txt_trim_space(char *str) { char *end; /* If str doesn't point to anything, just return the NULL pointer. */ if(str==NULL) return NULL; /* Remove the spaces before the start of the string. */ while(isspace(*str)) ++str; /* If there was nothing in the string, then just return the ending `\0' character. */ if(*str=='\0') return NULL; /* Remove the spaces at the end, and write a possibly new `\0'. */ end = str + strlen(str) - 1; while(end>str && isspace(*end)) --end; *(end+1)='\0'; /* Return the string. */ return *str=='\0' ? NULL : str; } /* Each information comment should have a format like this (replace `Column' with `Image' for 2D arrays): # Column N: NAME [UNITS, TYPE, BLANK] COMMENT TYPE has pre-defined values, and N must be an integer, but the rest can contain any characters (including whitespace characters). The UNITS, TYPE, BLANK tokens are optional, if not given, default values will be set. But if there are comments, then the brackets themselves are required to separate the name from the comments. Any white space characters before or after the delimiters (`:', `[', `]', `,') is ignored, but spaces within the values are kept. For example, in the two following lines, NAME will be set to `col name' (even though there are extra spaces in the second line, The column unit will be set to `col unit'. # Column 2: col name # Column 2 : col name [ col unit, type ] Column comments. When the column type is a string, the number of characters in the string is also necessary, for example `str10'. Without an integer attached, the line will be ignored. In the case of an error or mis-match, the line will be ignored. This function will make a linked list of information about each column that has information in the comments. The information on each column doesn't have to be in order, for example the information of column 10 can be before column 7. */ static void txt_info_from_comment(char *line, gal_data_t **datall, char *comm_start) { char *tailptr; gal_data_t *tmp; int index, strw=0; size_t len=strlen(comm_start); int type=GAL_TYPE_FLOAT64; /* Default type. */ char *number=NULL, *name=NULL, *comment=NULL; char *inbrackets=NULL, *unit=NULL, *typestr=NULL, *blank=NULL; /* Only read this comment line if it follows the convention: */ if( !strncmp(line, comm_start, len) ) { /* Set `name', `inbrackets', and `comment' in the first pass through the line. */ number=line+len; while(*line!='\0') { switch(*line) { case ':': if(name==NULL) { *line='\0'; name=line+1; } break; case '[': if(name && inbrackets==NULL) { *line='\0'; inbrackets=line+1; } break; case ']': if(inbrackets && comment==NULL) { *line='\0'; comment=line+1; } break; case '\n': *line='\0'; break; } ++line; } /* Read the column number as an integer. If it can't be read as an integer, or is zero or negative then just return without adding anything to this line. */ index=strtol(number, &tailptr, 0); if(*tailptr!='\0' || index<=0) return; /* If there was no name (the line is just `# Column N:'), then ignore the line. Relying on the column count from the first line is more robust and less prone to human error, for example typing a number larger than the total number of columns. */ name=txt_trim_space(name); if(name==NULL) return; /* If this is a repeated index, ignore it. */ for(tmp=*datall; tmp!=NULL; tmp=tmp->next) if(tmp->status==index) return; /* If there were brackets, then break it up. */ if(inbrackets) { unit=inbrackets; while(*inbrackets!='\0') { if(*inbrackets==',') { *inbrackets='\0'; if (typestr==NULL) typestr = inbrackets+1; else if(blank==NULL) blank = inbrackets+1; } ++inbrackets; } } /* If `typestr' was given, then check if this is a standard type. If `typestr' wasn't specified, then the default double type code will be used (see the variable definitions above). If the given type isn't a standard type then ignore the line. Just note that if we are dealing with the string type, we have to pull out the number part first. If there is no number for a string type, then ignore the line. */ if(typestr && *typestr!='\0') { typestr=txt_trim_space(typestr); if( !strncmp(typestr, "str", 3) ) { type=GAL_TYPE_STRING; strw=strtol(typestr+3, &tailptr, 0); if(*tailptr!='\0' || strw<0) return; } else { type=gal_type_from_name(typestr); if(type==GAL_TYPE_INVALID) return; } } /* Add this column's information into the columns linked list. We will define the data structur's array to have zero dimensions (no array) by default. If there is a blank value its value will be put into the array by `gal_table_read_blank'. To keep the name, unit, and comment strings, trim the white space before and after each before using them here. */ gal_list_data_add_alloc(datall, NULL, type, 0, NULL, NULL, 0, -1, name, txt_trim_space(unit), txt_trim_space(comment) ); /* Put the number of this column into the status variable of the data structure. If the type is string, then also copy the width into the structure. */ (*datall)->status=index; (*datall)->disp_width = type==GAL_TYPE_STRING ? strw : 0; /* Write the blank value into the array. Note that this is not the final column, we are just collecting information now. */ gal_tableintern_read_blank(*datall, txt_trim_space(blank)); } } /* In the case of a table, the input might not have had information in its comments, or the information might not have been complete. So we need to go through the first row of data also. In the case of the image, this is necessary, because we need to find the second dimension value. This function will return the number of tokens in the first row of the given text file. If the file is a text table with string columns, the contents of the string column will be counted as one token.*/ static size_t txt_info_from_first_row(char *line, gal_data_t **datall, int format) { gal_data_t *col, *prev, *tmp; size_t n=0, maxcnum=0, numtokens; char *token, *end=line+strlen(line); /* Remove the line termination character(s) from the end of the line. In Unix, the line terminator is just the new-line character, however, in some operating systems (like MS Windows), it is two characters: carriage return and new-line. To be able to deal with both, we will be checking the second last character first, the ASCII code for carriage return is 13. If the last column is a string, and the given length is larger than the available space on the line, we don't want to have the line's new-line character. Its better for it to actually be shorter than the space. */ if( *(end-2)==13 ) *(end-2)='\0'; else *(end-1)='\0'; /* Get the maximum number of columns read from the comment information. */ for(col=*datall; col!=NULL; col=col->next) maxcnum = maxcnum>col->status ? maxcnum : col->status; /* Go over the line check/fill the column information. */ while(++n) { /* When we are dealing with a text table, check if there is information for this column. For a text image, only the number of tokens is important (as the second dimension of the image), so just assume there no information. */ if(format==TXT_FORMAT_TABLE) for(col=*datall; col!=NULL; col=col->next) {if(col->status==n) break;} else col=NULL; /* If there is information for this column, then check if it is a string, and if so, don't use `strtok_r' (because it might have delimiters). So manually go ahead in the line till you get to the start of the string, then increment the line until the end of the space set for the strings. */ if(col) { if( col->type==GAL_TYPE_STRING ) { /* Remove all delimiters before the string starts. */ while(isspace(*line) || *line==',') ++line; /* Increment line to the end of the string. */ line = (token=line) + col->disp_width; /* If we haven't reached the end of the line, then set a NULL character where the string ends, so we can use the token. VERY IMPORTANT: this should not be `<=end'. If the given width is larger than line, there is no problem, the `\0' of the line will also be used to end this last column.*/ if(linestatus=n; } } } /* When looking at a text table, `n' is the number of columns (elements in the linked list). But when looking at an image, it is the size of the second dimension. To unify things from this step forwards, we will thus keep the value of `n' until this point in another variable (that will be returned finally), and for an image, change `n' to 1. This is necsesary in case the user has for example given two column information comments on an image plain text file. Note that `n' counts from 1, so the total number of tokens is one less than `n'.*/ numtokens=n-1; if(format==TXT_FORMAT_IMAGE) n=1; /* If the number of columns/images given by the comments is larger than the actual number of lines, remove those that have larger numbers from the linked list before things get complicated outside of this function. */ if(maxcnum>n) { prev=NULL; col=*datall; while(col!=NULL) { if(col->status > n) /* Column has no data (was only in comments) */ { /* This column has to be removed/freed. But we have to make some corrections before freeing it: - When `prev==NULL', then we still haven't got to the first valid element yet and must free this one, but if we do that, then the main pointer to the start of the list will be lost (we will loose all connections with the chain after leaving this loop). So we need to set that to the next element. - When there actually was a previous element (`prev!=NULL'), then we must correct it's next pointer. Otherwise we will break up the chain.*/ if(prev) prev->next=col->next; else *datall=col->next; tmp=col->next; gal_data_free(col); col=tmp; } else /* Column has data. */ { prev=col; col=col->next; } } } /* Return the total number of columns/second-img-dimension. */ return numtokens; } /* In the steps above, we read/set the information for each column. But to enforce minimum standard requirements on the user, things were allowed to be read very loosely, for example some columns can be not defined (and will thus be read as a double type), or they don't necessarily have to be given in the same order as the table (in which case, the first non-commented line provides basic information like how many columns there are). So we just pushed each new read/set column into a linked list. With this function, we convert that badly orderd linked list into a clean and ordered array for much more easier random access during the selection/reading of the data in the columns. After this function, the list is freed. */ static gal_data_t * txt_infoll_to_array(gal_data_t *datall, size_t *numdata) { size_t numc=0, ind; gal_data_t *data, *dataarr; /* First find the total number of columns. */ for(data=datall; data!=NULL; data=data->next) ++numc; /* Conversion to an arry is only necessary when there is more than one element in the list. */ if(numc>1) { /* Now, allocate the array and put in the values. */ dataarr=gal_data_array_calloc(numc); /* Put each dataset/column into its proper place in the array. */ while(datall!=NULL) { /* Pop the top element. */ data=gal_list_data_pop(&datall); /* The `status' value is the number of the column (counting from 1, not 0). */ ind=data->status-1; /* Put all the information from `data' into the respective part of the array. About the pointers, instead of having to allocate them again, we will just set them to NULL so `gal_data_free' doesn't remove them.*/ dataarr[ind].name = data->name; data->name=NULL; dataarr[ind].unit = data->unit; data->unit=NULL; dataarr[ind].array = data->array; data->array=NULL; dataarr[ind].dsize = data->dsize; data->dsize=NULL; dataarr[ind].comment = data->comment; data->comment=NULL; dataarr[ind].type = data->type; dataarr[ind].ndim = data->ndim; dataarr[ind].size = data->size; dataarr[ind].disp_width = data->disp_width; /* Clean up. */ gal_data_free(data); } } else dataarr=datall; /* Return the array of all column information and put the number of columns into the given pointer. */ *numdata=numc; return dataarr; } /* Return the information about a text file table. If there were no readable rows, it will return NULL.*/ static gal_data_t * txt_get_info(char *filename, int format, size_t *numdata, size_t *dsize) { FILE *fp; size_t numtokens; int firstlinedone=0; gal_data_t *datall=NULL, *dataarr; char *line, *format_err="empty", *comm_start; size_t linelen=10; /* `linelen' will be increased by `getline'. */ /* Set the constant strings */ switch(format) { case TXT_FORMAT_TABLE: format_err="table"; comm_start="# Column "; break; case TXT_FORMAT_IMAGE: format_err="image"; comm_start="# Image "; break; default: error(EXIT_FAILURE, 0, "%s: code %d not recognized", __func__, format); } /* Open the file. */ errno=0; fp=fopen(filename, "r"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s: couldn't open to read as a plain " "text %s in %s", filename, format_err, __func__); /* Allocate the space necessary to keep each line as we parse it. Note that `getline' is going to later `realloc' this space to fit the line length. */ errno=0; line=malloc(linelen*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for line", __func__, linelen*sizeof *line); /* Read the comments of the line for possible information about the lines, but also confirm/complete the info by parsing the first uncommented line. */ dsize[0]=0; while( getline(&line, &linelen, fp) != -1 ) switch( gal_txt_line_stat(line) ) { /* Line is a comment, see if it has formatted information. */ case GAL_TXT_LINESTAT_COMMENT: txt_info_from_comment(line, &datall, comm_start); break; /* Line is actual data, use it to fill in the gaps. */ case GAL_TXT_LINESTAT_DATAROW: ++dsize[0]; if(firstlinedone==0) { firstlinedone=1; numtokens=txt_info_from_first_row(line, &datall, format); if(format==TXT_FORMAT_IMAGE) dsize[1]=numtokens; } break; /* We also have the case of GAL_TXT_LINESTAT_BLANK. */ } /* The final dataset linked list can have any order (depending on how the user gave column information in tables for example). So here, we will convert the list into a nicely sorted array, note that this function frees list as part of the process. */ dataarr=txt_infoll_to_array(datall, numdata); /* Clean up. Note that even if there were no usable columns, there might have been meta-data comments, so we need to free `colsll' in any case. If the list is indeed empty, then `gal_data_free_ll' won't do anything. */ free(line); /* Close the file. */ errno=0; if(fclose(fp)) error(EXIT_FAILURE, errno, "%s: couldn't close file after reading plain " "text %s information in %s", filename, format_err, __func__); /* Return the array of column information. */ return dataarr; } /* Get the information of each column in a text file */ gal_data_t * gal_txt_table_info(char *filename, size_t *numcols, size_t *numrows) { return txt_get_info(filename, TXT_FORMAT_TABLE, numcols, numrows); } /* Get the information of a 2D array in a text file. */ gal_data_t * gal_txt_image_info(char *filename, size_t *numimg, size_t *dsize) { return txt_get_info(filename, TXT_FORMAT_IMAGE, numimg, dsize); } /************************************************************************/ /*************** Read a txt table ***************/ /************************************************************************/ static void txt_read_token(gal_data_t *data, gal_data_t *info, char *token, size_t i, char *filename, size_t lineno, size_t colnum) { char *tailptr; char **str = data->array, **strb; uint8_t *uc = data->array, *ucb; int8_t *c = data->array, *cb; uint16_t *us = data->array, *usb; int16_t *s = data->array, *sb; uint32_t *ui = data->array, *uib; int32_t *ii = data->array, *ib; uint64_t *ul = data->array, *ulb; int64_t *l = data->array, *lb; float *f = data->array, *fb; double *d = data->array, *db; /* Read the proper token into the column. */ switch(data->type) { case GAL_TYPE_STRING: gal_checkset_allocate_copy(txt_trim_space(token), &str[i]); if( (strb=info->array) && !strcmp( *strb, str[i] ) ) { free(str[i]); gal_checkset_allocate_copy(GAL_BLANK_STRING, &str[i]); } break; case GAL_TYPE_UINT8: uc[i]=strtol(token, &tailptr, 0); if( (ucb=info->array) && *ucb==uc[i] ) uc[i]=GAL_BLANK_UINT8; break; case GAL_TYPE_INT8: c[i]=strtol(token, &tailptr, 0); if( (cb=info->array) && *cb==c[i] ) c[i]=GAL_BLANK_INT8; break; case GAL_TYPE_UINT16: us[i]=strtol(token, &tailptr, 0); if( (usb=info->array) && *usb==us[i] ) us[i]=GAL_BLANK_UINT16; break; case GAL_TYPE_INT16: s[i]=strtol(token, &tailptr, 0); if( (sb=info->array) && *sb==s[i] ) s[i]=GAL_BLANK_INT16; break; case GAL_TYPE_UINT32: ui[i]=strtol(token, &tailptr, 0); if( (uib=info->array) && *uib==ui[i] ) ui[i]=GAL_BLANK_UINT32; break; case GAL_TYPE_INT32: ii[i]=strtol(token, &tailptr, 0); if( (ib=info->array) && *ib==ii[i] ) ii[i]=GAL_BLANK_INT32; break; case GAL_TYPE_UINT64: ul[i]=strtoul(token, &tailptr, 0); if( (ulb=info->array) && *ulb==ul[i] ) ul[i]=GAL_BLANK_UINT64; break; case GAL_TYPE_INT64: l[i]=strtol(token, &tailptr, 0); if( (lb=info->array) && *lb==l[i] ) l[i]=GAL_BLANK_INT64; break; /* For the blank value of floating point types, we need to make sure it isn't a NaN, because a NaN value will fail on any condition check (even `=='). If it isn't NaN, then we can compare the values. */ case GAL_TYPE_FLOAT32: f[i]=strtod(token, &tailptr); if( (fb=info->array) && ( (isnan(*fb) && isnan(f[i])) || *fb==f[i] ) ) f[i]=GAL_BLANK_FLOAT64; break; case GAL_TYPE_FLOAT64: d[i]=strtod(token, &tailptr); if( (db=info->array) && ( (isnan(*db) && isnan(d[i])) || *db==d[i] ) ) d[i]=GAL_BLANK_FLOAT64; break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, data->type); } /* If a number couldn't be read properly, then report an error. */ if(data->type!=GAL_TYPE_STRING && *tailptr!='\0') error_at_line(EXIT_FAILURE, 0, filename, lineno, "column %zu " "(`%s') couldn't be read as a `%s' number", colnum, token, gal_type_name(data->type, 1) ); } static void txt_fill(char *line, char **tokens, size_t maxcolnum, gal_data_t *info, gal_data_t *out, size_t rowind, char *filename, size_t lineno) { size_t i, n=0; gal_data_t *data; int notenoughcols=0; char *end=line+strlen(line); /* See explanations in `txt_info_from_first_row'. */ if( *(end-2)==13 ) *(end-2)='\0'; else *(end-1)='\0'; /* Start parsing the line. Note that `n' and `maxcolnum' start from one. */ while(++n) { /* Break out of the parsing if we don't need the columns any more. The table might contain many more columns, but when they aren't needed, there is no point in tokenizing them. */ if(n>maxcolnum) break; /* Set the pointer to the start of this token/column. See explanations in `txt_info_from_first_row'. */ if( info[n-1].type == GAL_TYPE_STRING ) { /* Remove any delimiters and stop at the first non-delimiter. If we have reached the end of the line then its an error, because we were expecting a column here. */ while(isspace(*line) || *line==',') ++line; if(*line=='\0') {notenoughcols=1; break;} /* Everything is good, set the pointer and increment the line to the end of the allocated space for this string. */ line = (tokens[n]=line) + info[n-1].disp_width; if(linestatus-1]') is not NULL and points to the blank value. For strings, this will actually be a string. */ switch(out->ndim) { case 1: for(data=out; data!=NULL; data=data->next) txt_read_token(data, &info[data->status-1], tokens[data->status], rowind, filename, lineno, data->status); break; case 2: for(i=0;idsize[1];++i) txt_read_token(out, info, tokens[i+1], rowind * out->dsize[1] + i, filename, lineno, i+1); break; default: error(EXIT_FAILURE, 0, "%s: currently only 1 and 2 dimensional " "datasets acceptable", __func__); } } static gal_data_t * gal_txt_read(char *filename, size_t *dsize, gal_data_t *info, gal_list_sizet_t *indexll, int minmapsize, int format) { FILE *fp; char *line; char **tokens; gal_data_t *out=NULL; gal_list_sizet_t *ind; size_t maxcolnum=0, rowind=0, lineno=0, ndim; size_t linelen=10; /* `linelen' will be increased by `getline'. */ /* Open the file. */ errno=0; fp=fopen(filename, "r"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s: couldn't open to read as a text table " "in %s", filename, __func__); /* Allocate the space necessary to keep a copy of each line as we parse it. Note that `getline' is going to later `realloc' this space to fit the line length. */ errno=0; line=malloc(linelen*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `line'", __func__, linelen*sizeof *line); /* Allocate all the desired columns for output. We will be reading the text file line by line, and writing in the necessary values of each row individually. */ switch(format) { /* This is a table. */ case TXT_FORMAT_TABLE: for(ind=indexll; ind!=NULL; ind=ind->next) { ndim=1; maxcolnum = maxcolnum>ind->v+1 ? maxcolnum : ind->v+1; gal_list_data_add_alloc(&out, NULL, info[ind->v].type, ndim, dsize, NULL, 0, minmapsize, info[ind->v].name, info[ind->v].unit, info[ind->v].comment); out->disp_width=info[ind->v].disp_width; out->status=ind->v+1; } break; /* This is an image. */ case TXT_FORMAT_IMAGE: if(info->next) error(EXIT_FAILURE, 0, "%s: currently reading only one image (2d " "array) from a text file is possible, the `info' input has " "more than one element", __func__); ndim=2; maxcolnum=dsize[1]; out=gal_data_alloc(NULL, info->type, ndim, dsize, NULL, 0, minmapsize, info->name, info->unit, info->comment); break; /* Not recognized. */ default: error(EXIT_FAILURE, 0, "%s: format code %d not recognized", __func__, format); } /* Allocate the space to keep the pointers to each token in the line. This is done here to avoid having to allocate/free this array for each line in `txt_fill_columns'. Note that the column numbers are counted from one (unlike indexes that are counted from zero), so we need `maxcolnum+1' elements in the array of tokens.*/ errno=0; tokens=malloc((maxcolnum+1)*sizeof *tokens); if(tokens==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `tokens'", __func__, (maxcolnum+1)*sizeof *tokens); /* Read the data columns. */ while( getline(&line, &linelen, fp) != -1 ) { ++lineno; if( gal_txt_line_stat(line) == GAL_TXT_LINESTAT_DATAROW ) txt_fill(line, tokens, maxcolnum, info, out, rowind++, filename, lineno); } /* Clean up and close the file. */ errno=0; if(fclose(fp)) error(EXIT_FAILURE, errno, "%s: couldn't close file after reading ASCII " "table information in %s", filename, __func__); free(tokens); free(line); /* Return the array of column information. */ return out; } gal_data_t * gal_txt_table_read(char *filename, size_t numrows, gal_data_t *colinfo, gal_list_sizet_t *indexll, size_t minmapsize) { return gal_txt_read(filename, &numrows, colinfo, indexll, minmapsize, TXT_FORMAT_TABLE); } gal_data_t * gal_txt_image_read(char *filename, size_t minmapsize) { size_t numimg, dsize[2]; gal_data_t *img, *imginfo; gal_list_sizet_t *indexll=NULL; /* Get the image information. */ imginfo=gal_txt_image_info(filename, &numimg, dsize); /* Read the table. */ img=gal_txt_read(filename, dsize, imginfo, indexll, minmapsize, TXT_FORMAT_IMAGE); /* Clean up and return. */ gal_data_free(imginfo); return img; } /************************************************************************/ /*************** Write to txt ***************/ /************************************************************************/ /* Make an array of 3 strings for each column (in practice a two dimensional array with 3 columns in a row for each input column). The columns are: Column 0: Printf format string. Column 1: Gnuastro type string (in plain text format). Column 2: Blank value string. */ #define FMTS_COLS 3 static char ** make_fmts_for_printf(gal_data_t *datall, int leftadjust, size_t *len) { char **fmts; gal_data_t *data; size_t i=0, num=0; char fmt[2], lng[3]; /* Allocate space for the output. */ for(data=datall;data!=NULL;data=data->next) ++num; errno=0; fmts=malloc(FMTS_COLS*num*sizeof *fmts); if(fmts==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for fmts", __func__, FMTS_COLS*num*sizeof *fmts); /* Initialize the length to 0. */ *len=0; /* Go over all the columns and make their formats. */ for(data=datall;data!=NULL;data=data->next) { /* First allocate the necessary space to keep the string. */ errno=0; fmts[ i*FMTS_COLS ] = malloc(GAL_TXT_MAX_FMT_LENGTH*sizeof **fmts); fmts[ i*FMTS_COLS+1 ] = malloc(GAL_TXT_MAX_FMT_LENGTH*sizeof **fmts); if(fmts[i*FMTS_COLS]==NULL || fmts[i*FMTS_COLS+1]==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for fmts[%zu] " "or fmts[%zu]", __func__, GAL_TXT_MAX_FMT_LENGTH*sizeof **fmts, i*FMTS_COLS, i*FMTS_COLS+1); /* If we have a blank value, get the blank value as a string and adjust the width */ fmts[ i*FMTS_COLS+2 ] = ( gal_blank_present(data, 0) ? gal_blank_as_string(data->type, 0) : NULL ); /* Fill in the printing paramters. */ gal_tableintern_col_print_info(data, GAL_TABLE_FORMAT_TXT, fmt, lng); /* Adjust the width if a blank string was defined. */ if(fmts[i*FMTS_COLS+2]) data->disp_width = ( strlen(fmts[i*FMTS_COLS+2]) > data->disp_width ? strlen(fmts[i*FMTS_COLS+2]) : data->disp_width ); /* Print the result into the allocated string and add its length to the final length of the overall format statement. The space in the end of `fmts[i*2]' is to ensure that the columns don't merge, even if the printed string is larger than the expected width. */ if(data->disp_precision > 0) *len += 1 + sprintf(fmts[i*FMTS_COLS], "%%%s%d.%d%s%s ", leftadjust ? "-" : "", data->disp_width, data->disp_precision, lng, fmt); else *len += 1 + sprintf(fmts[i*FMTS_COLS], "%%%s%d%s%s ", leftadjust ? "-" : "", data->disp_width, lng, fmt); /* Set the string for the Gnuastro type. For strings, we also need to write the maximum number of characters.*/ if(data->type==GAL_TYPE_STRING) sprintf(fmts[i*FMTS_COLS+1], "%s%d", gal_type_name(data->type, 0), data->disp_width); else strcpy(fmts[i*FMTS_COLS+1], gal_type_name(data->type, 0)); /* Increment the column counter. */ ++i; } /* Return the array. */ return fmts; } static void txt_print_value(FILE *fp, void *array, int type, size_t ind, char *fmt) { switch(type) { /* Numerical types. */ case GAL_TYPE_UINT8: fprintf(fp, fmt, ((uint8_t *) array)[ind]); break; case GAL_TYPE_INT8: fprintf(fp, fmt, ((int8_t *) array)[ind]); break; case GAL_TYPE_UINT16: fprintf(fp, fmt, ((uint16_t *)array)[ind]); break; case GAL_TYPE_INT16: fprintf(fp, fmt, ((int16_t *) array)[ind]); break; case GAL_TYPE_UINT32: fprintf(fp, fmt, ((uint32_t *)array)[ind]); break; case GAL_TYPE_INT32: fprintf(fp, fmt, ((int32_t *) array)[ind]); break; case GAL_TYPE_UINT64: fprintf(fp, fmt, ((uint64_t *)array)[ind]); break; case GAL_TYPE_INT64: fprintf(fp, fmt, ((int64_t *) array)[ind]); break; case GAL_TYPE_FLOAT32: fprintf(fp, fmt, ((float *) array)[ind]); break; case GAL_TYPE_FLOAT64: fprintf(fp, fmt, ((double *) array)[ind]); break; /* Special consideration for strings. */ case GAL_TYPE_STRING: if( !strcmp( ((char **)array)[ind], GAL_BLANK_STRING ) ) fprintf(fp, fmt, GAL_BLANK_STRING); else fprintf(fp, fmt, ((char **)array)[ind]); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } } static FILE * txt_open_file_write_info(gal_data_t *datall, char **fmts, gal_list_str_t *comment, char *filename) { FILE *fp; gal_data_t *data; char *tmp, *nstr; size_t i, j, num=0; gal_list_str_t *strt; int nlen, nw=0, uw=0, tw=0, bw=0; /* Make sure the file doesn't already eixist. */ if( gal_checkset_check_file_return(filename) ) error(EXIT_FAILURE, 0, "%s: %s already exists. For safety, this " "function will not over-write an existing file. Please delete " "it before calling this function", __func__, filename); /* Open the output file. */ errno=0; fp=fopen(filename, "w"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s: couldn't be open to write text " "table by %s", filename, __func__); /* Write the comments if there were any. */ for(strt=comment; strt!=NULL; strt=strt->next) fprintf(fp, "# %s\n", strt->v); /* Get the maximum width for each information field. */ for(data=datall;data!=NULL;data=data->next) { ++num; if( data->name && strlen(data->name)>nw ) nw=strlen(data->name); if( data->unit && strlen(data->unit)>uw ) uw=strlen(data->unit); } for(i=0;i tw ? strlen(tmp) : tw; if( (tmp=fmts[ i*FMTS_COLS+2 ]) ) /* If it isn't NULL. */ bw = strlen(tmp) > bw ? strlen(tmp) : bw; } /* Write the column information if the output is a file. When the output is directed to standard output (the command-line), it is most probably intended for piping into another program (for example AWK for further processing, or sort, or anything) so the user already has the column information and is probably going to change them, so they are just a nuisance. When there are more than 9 columns, we don't want to have cases like `# Column 1 :' (note the space between `1' and `:', this space won't exist for the 2 digit colum numbers). To do this, we are first allocating and printing a string long enough to keep the final column's `N:'. Then, for each column, we print only the number into the allocated space and put the `:' in manually immediately after the number. Note that the initial `asprintf' put a `\0' in the allocated space, so we can safely over-write the one that `sprintf' puts with a `:' for the columns that have the same number of digits as the final column. */ i=0; asprintf(&nstr, "%zu:", num); nlen=strlen(nstr); for(data=datall; data!=NULL; data=data->next) { /* Print the number into the number string, then add the `:' immediately after the number. */ sprintf(nstr, "%zu", i+1); for(j=1;jndim==1 ? "Column" : "Image", nstr, nw, data->name ? data->name : "", uw, data->unit ? data->unit : "", tw, fmts[i*FMTS_COLS+1] ? fmts[i*FMTS_COLS+1] : "", bw, fmts[i*FMTS_COLS+2] ? fmts[i*FMTS_COLS+2] : "", data->comment ? data->comment : ""); ++i; } /* Clean up and return. */ free(nstr); return fp; } void gal_txt_write(gal_data_t *input, gal_list_str_t *comment, char *filename) { FILE *fp; char **fmts; size_t i, j, num=0, fmtlen; gal_data_t *data, *next2d=NULL; /* Make sure input is valid. */ if(input==NULL) error(EXIT_FAILURE, 0, "%s: input is NULL", __func__); /* Currently only 1 and 2 dimension datasets are acceptable. */ if( input->ndim!=1 && input->ndim!=2 ) error(EXIT_FAILURE, 0, "%s: only 1 and 2 dimensional datasets are " "currently supported. The input dataset has %zu dimensions", __func__, input->ndim); /* For a 2D dataset, we currently don't accept a list, we can only print one column. So keep the next pointer separately and restore it after the job of this function is finished. */ if(input->ndim==2) { next2d=input->next; input->next=NULL; } /* Find the number of columns, do a small sanity check, and get the maximum width of the name and unit string if they are present. */ for(data=input;data!=NULL;data=data->next) { /* Count. */ ++num; /* Check if the dimensionality and size is the same for all the elements. */ if( input!=data && gal_data_dsize_is_different(input, data) ) error(EXIT_FAILURE, 0, "%s: the input list of datasets must have the " "same sizes (dimentionality and length along each dimension)", __func__); } /* Prepare the necessary formats for each column, then allocate the space for the full list and concatenate all the separate inputs into it. */ fmts=make_fmts_for_printf(input, 1, &fmtlen); /* Set the output FILE pointer: if it isn't NULL, its an actual file, otherwise, its the standard output. */ fp = ( filename ? txt_open_file_write_info(input, fmts, comment, filename) : stdout ); /* Print the dataset */ switch(input->ndim) { case 1: for(i=0;isize;++i) /* Row. */ { j=0; for(data=input;data!=NULL;data=data->next) /* Column. */ txt_print_value(fp, data->array, data->type, i, fmts[j++ * FMTS_COLS]); fprintf(fp, "\n"); } break; case 2: for(i=0;idsize[0];++i) { for(j=0;jdsize[1];++j) txt_print_value(fp, input->array, input->type, i*input->dsize[1]+j, fmts[0]); fprintf(fp, "\n"); } break; default: error(EXIT_FAILURE, 0, "%s: a bug! input->ndim=%zu is not recognized", __func__, input->ndim); } /* Clean up. */ for(i=0;indim==2) input->next=next2d; } gnuastro-0.5/lib/timing.c0000644000175000017500000000423213121462410012335 00000000000000/********************************************************************* Functions to report timing in verbose mode. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include /* Micro-second based timer, which can be used to generate random numbers. The type of `tv_sec' and `tv_usec' is `long int' (from the GNU C Library manual), so this function will also return long. */ long gal_timing_time_based_rng_seed() { struct timeval tv; gettimeofday(&tv,0); return tv.tv_sec + tv.tv_usec; } /* Used to report the time it takes for an action to be done. */ void gal_timing_report(struct timeval *t1, char *jobname, size_t level) { double dt=1e30; struct timeval t2; if(t1) { gettimeofday(&t2, NULL); dt= ( ((double)t2.tv_sec+(double)t2.tv_usec/1e6) - ((double)t1->tv_sec+(double)t1->tv_usec/1e6) ); } if(level==0) printf("%s %-f seconds\n", jobname, dt); else if(level==1) { if(t1) printf(" - %-*s %f seconds\n", GAL_TIMING_VERB_MSG_LENGTH_V, jobname, dt); else printf(" - %s\n", jobname); } else if(level==2) { if(t1) printf(" ---- %-*s %f seconds\n", GAL_TIMING_VERB_MSG_LENGTH_V-3, jobname, dt); else printf(" ---- %s\n", jobname); } } gnuastro-0.5/lib/tile.c0000644000175000017500000012506113161316532012016 00000000000000/********************************************************************* tile -- work with tesselations over a host dataset. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /***********************************************************************/ /************** Single tile ******************/ /***********************************************************************/ /* Calculate the starting coordinates of a tile in the allocated block of memory. */ void gal_tile_start_coord(gal_data_t *tile, size_t *start_coord) { size_t ind, ndim=tile->ndim; gal_data_t *block=gal_tile_block(tile); /* If the input tile is actually the same as the block, then the start is at 0 (in all dimensions). */ if(block==tile) memset(start_coord, 0, ndim*gal_type_sizeof(GAL_TYPE_SIZE_T)); else { /* Calculate the coordinates of the first pixel of the tile. */ ind = gal_data_ptr_dist(block->array, tile->array, block->type); gal_dimension_index_to_coord(ind, ndim, block->dsize, start_coord); } } /* Put the starting and ending (end point is not inclusive) coordinates of a tile into the `start_end' array. It is assumed that a space of `2*tile->ndim' has been already allocated (static or dynamic) before this function is called. `rel_block' (or relative-to-block) is only relevant when the tile has an intermediate tile between it and the allocated space (like a channel, see `gal_tile_full_two_layers'). If it doesn't (`tile->block' points the allocated dataset), then the value to `rel_block' is irrelevant. However, when `tile->block' is its self a larger block and `rel_block' is set to 0, then the starting and ending positions will be based on the position within `tile->block', not the allocated space. */ void gal_tile_start_end_coord(gal_data_t *tile, size_t *start_end, int rel_block) { size_t *s, *sf, *h; gal_data_t *block=gal_tile_block(tile); gal_data_t *host=rel_block ? block : tile->block; size_t *hcoord, start_ind, ndim=tile->ndim, *end=start_end+ndim; /* Get the starting index. Note that for the type we need the allocated block dataset and can't rely on the tiles. */ start_ind=gal_data_ptr_dist(block->array, tile->array, block->type); /* Get the coordinates of the starting point relative to the allocated block. */ gal_dimension_index_to_coord(start_ind, ndim, block->dsize, start_end); /* When the host is different from the block, the tile's starting position needs to be corrected. */ if(host!=block) { /* Get the host's starting coordinates. */ start_ind=gal_data_ptr_dist(block->array, host->array, block->type); /* Temporarily put the host's coordinates in the place held for the ending coordinates. */ hcoord=end; gal_dimension_index_to_coord(start_ind, ndim, block->dsize, hcoord); sf=(s=start_end)+ndim; h=hcoord; do *s++ -= *h++; while(sdsize, end, ndim); } /* Put the indexs of the first/start and last/end pixels (inclusive) in a tile into the `start_end' array (that has two elements). It will then return the pointer to the start of the tile in the `work' data structure. */ void * gal_tile_start_end_ind_inclusive(gal_data_t *tile, gal_data_t *work, size_t *start_end_inc) { gal_data_t *block=gal_tile_block(tile); size_t ndim=tile->ndim, *s, *e, *l, *sf; size_t *start_coord = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "start_coord"); size_t *end_coord = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "end_coord"); /* The starting index can be found from the distance of the `tile->array' pointer and `block->array' pointer. IMPORTANT: with the type of the block array. */ start_end_inc[0]=gal_data_ptr_dist(block->array, tile->array, block->type); /* To find the end index, we need to know the coordinates of the starting point in the allocated block. */ gal_dimension_index_to_coord(start_end_inc[0], ndim, block->dsize, start_coord); /* `end_coord' is one unit ahead of the last element in the tile in every dimension. To have less potential for bugs, we will remove that extra value, so we get the coordinates of the last pixel in the tile (inclusive). We will finally, increment that value by one to get to the pixel immediately outside of the tile.*/ e=end_coord; l=tile->dsize; sf=(s=start_coord)+ndim; do *e++ = *s + *l++ - 1; while(++sdsize, end_coord); /* For a check: printf("\ntile_dsize: %zu, %zu, %zu\n", tile->dsize[0], tile->dsize[1], tile->dsize[2]); printf("start_coord: %zu, %zu, %zu\n", start_coord[0], start_coord[1], start_coord[2]); printf("end_coord: %zu, %zu, %zu\n", end_coord[0], end_coord[1], end_coord[2]); printf("start_index: %zu\n", start_end_inc[0]); printf("end_index: %zu\n", start_end_inc[1]); exit(1); */ /* Clean up and return the pointer in the work array that the tile starts from. */ free(end_coord); free(start_coord); return gal_data_ptr_increment(work->array, start_end_inc[0], work->type); } /***********************************************************************/ /************** Series of tiles ******************/ /***********************************************************************/ /* Construct a list of tile(s) given positional minimum(s) and maximum(s). The output is an allocated an allocated array that can later be freed with `gal_data_array_free'. The minimum and maximums are assumed to be inclusive. The array keeping the minmium and maximum coordinates for each label will have the following format: | min0_d0 | min0_d1 | max0_d0 | max0_d1 | ... ... | minN_d0 | minN_d1 | maxN_d0 | maxN_d1 | */ gal_data_t * gal_tile_series_from_minmax(gal_data_t *block, size_t *minmax, size_t number) { size_t ndim=block->ndim; size_t *min, *max; size_t i, d, ind, size, width=2*ndim; gal_data_t *tiles=gal_data_array_calloc(number); /* Fill the tile information. */ for(i=0;idsize, min); tiles[i].array = gal_data_ptr_increment(block->array, ind, block->type); } /* For a check (put all the objects in an extension of a test file). { gal_data_t *copy; for(i=0;iblock!=NULL) tile=tile->block; return tile; } /* Return the increment necessary to start at the next series of contiguous memory (fastest dimension) associated with a tile. 1D and 2D cases are simple and need no extra explanation, but the case for higher dimensions can be alittle more complicated, So we will go over some examples. The notations below are: `n' number of dimensions (same in tile and block). `t[]' size of the tile in each dimension. `b[]' size of the allocated block in each dimension. It is just important to see the output of this function as an increment from the the last patch of contiguous memory associated with the tile. So when the increment number is `t[n-1]' (the first 2D slice of the tile has been parsed), simply incrementing by `b[n-2] * b[n-1]' will take us to the last row of num_increment coord increment ------------- ----- --------- 1 (...0,0,0) b[n-1]: fastest dimension of the block. 2 (...0,1,0) Similar to previous . . . . . . t[n-2] (...1,0,0) (b[n-2] * b[n-1]) - ( (t[n-2]-1) * b[n-1] ) t[n-2] + 1 (...1,1,0) b[n-1] . . . . . . 2 * t[n-2] (...2,0,0) b[n-2] * b[n-1] t[n-2]+1 (...2,1,0) b[n-1] . . . . . . t[n-3] * t[n-2] (..1,0,0,0) b[n-3] * b[n-2] * b[n-1] */ size_t gal_tile_block_increment(gal_data_t *block, size_t *tsize, size_t num_increment, size_t *coord) { size_t n=block->ndim; size_t *b=block->dsize, *t=tsize; size_t increment=GAL_BLANK_SIZE_T; if(n>3) error(EXIT_FAILURE, 0, "%s: currently only implemented for at most 3 " "dimensions", __func__); switch(n) { /* A zero-dimensional dataset is not defined. */ case 0: error(EXIT_FAILURE, 0, "%s: zero dimensional input is not acceptable", __func__); /* 1D: the increment is just the tile size. */ case 1: increment=t[0]; if(coord) coord[0]+=increment; break; /* 2D: the increment is the block's number of fastest axis pixels. */ case 2: increment=b[1]; if(coord) ++coord[0]; break; /* 3D: The increment depends on which dimension we are reaching. */ case 3: if(num_increment % t[1]) { increment = b[2]; if(coord) ++coord[1]; } else { increment=(b[1] * b[2]) - ( (t[1]-1) * b[2] ); if(coord) { ++coord[0]; coord[1] -= t[1]-1; coord[2]=0; } } break; } /* Return the final increment value. */ return increment; } /* Write a constant value for each tile into each pixel covered by the input tiles in an array the size of the block and return it. Arguments --------- `tilevalues': This must be an array that has the same number of elements as that in `tilesll' and in the same order that `tilesll' elements are parsed (from first to last). As a result the dimensionality of this array is irrelevant. Note that unlike `tiles', `tilevalues' must be an array. `tilesll': This will be parsed as a linked list (using the `next' element). Internally, it might be stored as an array, but this function doesn't care! The position of the tile over its block will be determined according to the `block' element and the pointer of its `array' as fully described in `gnuastro/data.h'. This function will not pop/free the list, it will only parse it from start to end. `initialize': Initialize the allocated space with blank values before writing in the constant values. This can be useful when the tiles don't cover the full allocated block. */ gal_data_t * gal_tile_block_write_const_value(gal_data_t *tilevalues, gal_data_t *tilesll, int withblank, int initialize) { void *in; int type=tilevalues->type; size_t tile_ind, nt=0, nv=tilevalues->size; gal_data_t *tofill, *tile, *block=gal_tile_block(tilesll); /* A small sanity check. */ for(tile=tilesll; tile!=NULL; tile=tile->next) ++nt; if(nt!=nv) error(EXIT_FAILURE, 0, "%s: the number of elements in `tilevalues' (%zu) " "and `tilesll' (%zu) must be the same", __func__, nv, nt); /* Allocate the output array. */ tofill=gal_data_alloc(NULL, type, block->ndim, block->dsize, block->wcs, 0, block->minmapsize, tilevalues->name, tilevalues->unit, tilevalues->comment); /* If requested, initialize `tofill', otherwise it is assumed that the full area of the output is covered by the tiles. */ if(withblank || initialize) gal_blank_initialize(tofill); else { /* Copy the flags. */ tofill->flag=tilevalues->flag; /* If we have more than one dimension, then remove the possibly sorted flags. */ if(block->ndim>1) { tofill->flag &= ~GAL_DATA_FLAG_SORTED_I; tofill->flag &= ~GAL_DATA_FLAG_SORTED_D; } } /* Go over the tiles and write the values in. Recall that `tofill' has the same type as `tilevalues'. So we are using memcopy. */ tile_ind=0; for(tile=tilesll; tile!=NULL; tile=tile->next) { /* Set the pointer to use as input. The `if(o)' statement is set because GCC 7.1.1 complained about the possiblity of the first argument of `memcpy' being NULL. Recall that `o' is a pointer. */ in=gal_data_ptr_increment(tilevalues->array, tile_ind++, type);; GAL_TILE_PARSE_OPERATE( tile, tofill, 1, withblank, { if(o) memcpy(o, in, gal_type_sizeof(type)); } ); } return tofill; } /* Make a copy of the memory block and fill it with the index of each tile in `tilesll' (counting from 0). The non-filled areas will have blank values. The output dataset will have a type of `GAL_TYPE_INT32'. */ gal_data_t * gal_tile_block_check_tiles(gal_data_t *tilesll) { int32_t *arr; size_t i, dsize=gal_list_data_number(tilesll); gal_data_t *ids, *out, *block=gal_tile_block(tilesll); /* Allocate the array to keep the IDs of each tile. */ ids=gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &dsize, NULL, 0, block->minmapsize, NULL, NULL, NULL); /* Put the IDs into the array. */ arr=ids->array; for(i=0;iarray, gal_data_ptr_dist(block->array, tile->array, block->type), other->type); } /* To use within `gal_tile_full_blank_flag'. */ static void * tile_block_blank_flag(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; gal_data_t *tile_ll=(gal_data_t *)(tprm->params); size_t i; gal_data_t *tile; /* Check all the tiles given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { tile=&tile_ll[ tprm->indexs[i] ]; gal_blank_present(tile, 1); } /* Wait for all the other threads to finish. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* Update the blank flag on the tiles within the list of input tiles. */ void gal_tile_block_blank_flag(gal_data_t *tile_ll, size_t numthreads) { /* Go over all the tiles and update their blank flag. */ gal_threads_spin_off(tile_block_blank_flag, tile_ll, gal_list_data_number(tile_ll), numthreads); } /***********************************************************************/ /************** Tile full dataset ********************/ /***********************************************************************/ /* The user's specified tile size might not be an exact multiple of the parent's size. This function is useful in such cases. It will give the starting tile's size along each dimension. The line below can be the length along any dimension and the tile size along that dimension. You see that when we start with the tile size, we will end up with a last tile that contains the remainder elements. | tile size | tile size | tile size | tile size | remainder | | | | | | --------------------------------------------------------- The remainder will always be smaller than `tile size'. So, we will merge the last tile size with the remainder and move that tile to the start. In this way, the size of the first tile will always be between between one and two times the size of the regular tile: | first tile | tile size | tile size | tile size | | | | | | --------------------------------------------------------- When there is only a small remainder (for example one or two pixels), then this layout is fine. But when the remainder is significant compared to the regular tile size (like the example above), then it will make more sense to cut the first tile into two halfs (`f-half' and `l-half') and put them at the start and end of the full length: | f-half | tile size | tile size | tile size | l-half | | | | | | | --------------------------------------------------------- So in any case, knowing the size of the first tile, will allow us to parse all the tiles. We just have to make sure we don't go over the full input's length. */ static void gal_tile_full_regular_first(gal_data_t *parent, size_t *regular, float remainderfrac, size_t *first, size_t *last, size_t *tsize) { size_t i, remainder, *dsize=parent->dsize;; /* For each dimension, set the size of the first tile. */ for(i=0;indim;++i) { /* It might happen that the tile size is bigger than the parent size in a dimension, in that case the analysis in the comments above are useless and only one tile should cover this dimension with the size of the parent. */ if( regular[i] >= dsize[i] ) { tsize[i]=1; first[i]=last[i]=dsize[i]; } else { /* Calculate the remainder in this dimension. */ remainder=dsize[i] % regular[i]; /* Depending on the remainder, set the first tile size and number. */ if(remainder) { if( remainder > remainderfrac * regular[i] ) { first[i] = ( remainder + regular[i] )/2; tsize[i] = dsize[i]/regular[i] + 1 ; last[i] = ( dsize[i] - ( first[i] + regular[i]*(tsize[i]-2) ) ); } else { first[i] = remainder + regular[i]; tsize[i] = dsize[i]/regular[i]; last[i] = regular[i]; } } else { first[i] = last[i] = regular[i]; tsize[i] = dsize[i]/regular[i]; } } } } /* Cover the full dataset with (mostly) identical tiles. The regular tile size is determined from the `size' array. If the input data's size is not an exact multiple of `size' for each dimension, then the tiles touching the edges in that dimension will have a different size to fully cover every element of the input. For a full description of tiling in `gal_data_t', please see `data.h'. Inputs ------ `input' is the gal_data_t which you want to tile (only used for its sizes). `regular' is the size of the regular tiles along each of the input's dimensions. So it must have the same number of elements as the dimensions of `input'. `remainderfrac' is the significant fraction of the remainder space if the width of the input isn't an exact multiple of the tile size along a dimension, see `gal_tile_full_regular_first'. `out' is the pointer to the array of data structures that is to keep the tile parameters. If `*out==NULL', then the necessary space will be allocated. If it is not NULL, then all the tile information will be filled from the given element, see `multiple' for more. `multiple': When the `*out' array is to be allocated, allocate `multiple' times the necessary space. This can be very useful when you have several more identically sized `inputs', and you want all their tiles to be allocated (and thus indexed) together, even though they have different `block' datasets (that then link to one allocated space). See the `gal_tile_full_two_layers' below. `firsttsize': The size of the first tile along every dimension. This is only different from the regular tile size when `regular' is not an exact multiple of `input''s length along every dimension. This array is allocated internally by this function. Output ------ The returned output is an array of numbers (the same size as the input data structure's dimensions) keeping the number of tiles along each dimension. Implementation -------------- In the most general case, to set the starting pointers for each tile we need the following sizes. If the input array has no parent/block, then both these sizes are equal to it's own size: 1. block-size (or `bsize'), which is the size of the allocated block in each dimension. 2. parent-size (or `psize') which is the size of the parent in each dimension (we don't want to go out of the paren't range). */ size_t * gal_tile_full(gal_data_t *input, size_t *regular, float remainderfrac, gal_data_t **out, size_t multiple, size_t **firsttsize) { size_t i, d, tind, numtiles, *start=NULL; gal_data_t *tiles, *block=gal_tile_block(input); size_t *last = gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim, __func__, "last"); size_t *first = gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim, __func__, "first"); size_t *coord = gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim, __func__, "coord"); size_t *tcoord = gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim, __func__, "tcoord"); size_t *tsize = gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim+1, __func__, "tsize"); /* Set the first tile size and total number of tiles along each dimension, then allocate the array of tiles. */ gal_tile_full_regular_first(input, regular, remainderfrac, first, last, tsize); numtiles=gal_dimension_total_size(input->ndim, tsize); /* Allocate the necessary space for all the tiles (if necessary). */ if(*out) tiles = *out; else *out = tiles = gal_data_array_calloc(numtiles*multiple); /* It is possible that the `input' dataset is its-self a larger tile over a region of the allocated block. In that case, we need to account for the block's dimensions when calculating the position of this block. */ if(input->block) { start=gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim, __func__, "start"); gal_tile_start_coord(input, start); } /* Initialize each tile. */ for(i=0;indim, tsize, tcoord); /* The coordinates are currently in units of tiles, not pixels. Convert them to the coordinates of the first pixel in each tile. */ for(d=0;dndim;++d) { /* Convert the tile coordinates to pixel coordinates within `input'. See the comments above `gal_tile_full_regular_first': The first tile in every dimension can be different from the regular tile size. */ coord[d] = tcoord[d] ? first[d] + (tcoord[d]-1)*regular[d] : 0; /* When the `input' data structure (that is to be tiled here) was itself a tile over a larger allocated array, a `start' array has been allocated to correct the coordinates so they refer to a physical position on the allocated block of memory. */ if(start) coord[d] += start[d]; } /* Convert the coordinates (that are now in element/pixel units on the allocated block of memory) into an index. */ tind=gal_dimension_coord_to_index(block->ndim, block->dsize, coord); /* Now that we have the index of this tile's starting point compared to the allocated block, put it in to the tile's `array' pointer. */ tiles[i].array=gal_data_ptr_increment(block->array, tind, block->type); /* Set the sizes of the tile. */ tiles[i].size=1; /* Just an initializer, will be changed. */ tiles[i].ndim=input->ndim; tiles[i].minmapsize=input->minmapsize; tiles[i].dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T,input->ndim, __func__, "tiles[i].dsize"); for(d=0;dndim;++d) { /* The size of the first and last tiles can be different from the majority of the `regular' tiles that have the same size. When a tile is on the edge in one of the dimensions, then its `coord[d]' will be either 0 or the last. */ if( first[d] != regular[d] && ( tcoord[d]==0 || tcoord[d]==tsize[d]-1 ) ) { if( tcoord[d] == 0 ) tiles[i].dsize[d] = first[d]; if( tcoord[d] == tsize[d]-1 ) tiles[i].dsize[d] = last[d]; } else tiles[i].dsize[d]=regular[d]; /* Set the size value. */ tiles[i].size *= tiles[i].dsize[d]; } /* Set the block structure for this tile to the `input', and set the next pointer as the next tile. Note that only when we are dealing with the last tile should the `next' pointer be set to NULL.*/ tiles[i].flag = 0; tiles[i].block = input; tiles[i].next = i==numtiles-1 ? NULL : &tiles[i+1]; /* For a check: printf("%zu:\n\tStart index: %zu\n\tsize: %zu x %zu\n", i, tind, tiles[i].dsize[1], tiles[i].dsize[0]); exit(0); */ } /* Clean up and return. */ free(last); free(coord); free(tcoord); *firsttsize=first; if(start) free(start); tsize[input->ndim]=-1; /* `tsize' had ndim+1 values, we will mark the */ return tsize; /* extra space with the largest possible value: */ } /* -1, see `gal_tile_full_sanity_check'. */ /* Make sure that the input parameters (in `tl', short for two-layer) fit with the input dataset. The filename and HDU are only required for error messages. Also, allocate and fill the `channelsize' array. */ void gal_tile_full_sanity_check(char *filename, char *hdu, gal_data_t *input, struct gal_tile_two_layer_params *tl) { double d; size_t i, ndim=input->ndim; /* Check the tile's dimensions. */ for(i=0;tl->tilesize[i]!=-1;++i) { /* Not equal to zero. */ if(tl->tilesize[i]==0) error(EXIT_FAILURE, 0, "`--tilesize' must be larger than zero, " "the given value for dimension %zu was zero", ndim-i); /* If the tile size is larger than the dataset size in this dimension, then quietly change the tile size to the dataset size along that dimension. */ if( tl->tilesize[i] > input->dsize[i] ) tl->tilesize[i] = input->dsize[i]; } /* Make sure the number of tile sizes (tile dimensions) are the same as the dataset's dimensions). */ if(i!=ndim) error(EXIT_FAILURE, 0, "%s (hdu: %s): has %zu dimensions, but only %zu " "value(s) given for the tile size (`--tilesize' option).", filename, hdu, ndim, i); /* Check the channel's dimensions. */ for(i=0; tl->numchannels[i]!=-1; ++i) if(tl->numchannels[i]==0) error(EXIT_FAILURE, 0, "the number of channels in all dimensions must " "be larger than zero. The number for dimension %zu was zero", i+1); if(i!=ndim) error(EXIT_FAILURE, 0, "%s (hdu: %s): has %zu dimensions, but only %zu " "value(s) given for the number of channels", filename, hdu, ndim, i); /* Allocate space for the channel sizes. */ tl->channelsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "tl->channelsize"); /* Check if the channels are exactly divisible by the input's size along each dimension and set the correct size. */ for(i=0;idsize[i] < tl->numchannels[i] ) error(EXIT_FAILURE, 0, "the number of channels in dimension %zu " "(%zu) is more than the size of the `%s' (hdu: %s) in that " "dimension", ndim-i, tl->numchannels[i], filename, hdu); /* Also check the tile size. */ if( input->dsize[i] < tl->tilesize[i] ) error(EXIT_FAILURE, 0, "the tile size in dimension %zu (%zu) is " "more than the size of the `%s' (hdu: %su) in that dimension", ndim-i, tl->tilesize[i], filename, hdu); /* First check. */ d=(double)input->dsize[i]/(double)(tl->numchannels[i]); if(ceil(d)!=d) error(EXIT_FAILURE, 0, "%zu (number of channels along dimension " "%zu) is not exactly divisible by %zu (the length of `%s' " "(hdu: %s) that dimension). The channels cover the input " "dataset, hence, they must be identical", tl->numchannels[i], ndim-i, input->dsize[i], filename, hdu); /* Put the channel size into the output. */ tl->channelsize[i]=d; } } /* A dataset can be tiled with two layers that are related: Channels: A tesselation of larger tile sizes that all have the same size (`channel_size' must be an exact multiple of `input's size along every dimension. In astronomy images, this can be seen as CCD amplifiers, that cover large parts of the image. If `*channels!=NULL' then it is assumed to be already present and will not be allocated. Tiles: A combined tesselation of each channel with smaller tiles. These tiles can be used to calculate things like gradients over each channel and thus over the whole image. */ void gal_tile_full_two_layers(gal_data_t *input, struct gal_tile_two_layer_params *tl) { gal_data_t *t; size_t i, *junk, *junk2, ndim=tl->ndim=input->ndim; /* Initialize. */ tl->channels=tl->tiles=NULL; /* Initialize necessary values and do the channels tessellation. */ junk = gal_tile_full(input, tl->channelsize, tl->remainderfrac, &tl->channels, 1, &junk2); tl->totchannels = gal_dimension_total_size(ndim, tl->numchannels); for(i=0;inumchannels[i]) error(EXIT_FAILURE, 0, "%s: the input and output number of channels " "don't match in dimension %zu: %zu and %zu respectively.", __func__, ndim-i, tl->numchannels[i], junk[i]); free(junk); free(junk2); /* Tile each channel. While tiling the first channel, we are also going to allocate the space for the other channels. Then pass those pointers when we want to fill in each tile of the other channels. */ tl->numtilesinch = gal_tile_full(tl->channels, tl->tilesize, tl->remainderfrac, &tl->tiles, tl->totchannels, &tl->firsttsize); tl->tottilesinch = gal_dimension_total_size(ndim, tl->numtilesinch); for(i=1; itotchannels; ++i) { /* Set the first tile in this channel. Then use it it fill the `next' pointer of the previous channel's tiles. Note that `gal_tile_full' set this `next' element to NULL. */ t = tl->tiles + i * tl->tottilesinch; tl->tiles[ i * tl->tottilesinch - 1 ].next = t; /* Fill in the information for all the tiles in this channel. Note that we already have the returned value, so it isn't important.*/ junk=gal_tile_full(&tl->channels[i], tl->tilesize, tl->remainderfrac, &t, 1, &junk2); free(junk); free(junk2); } /* Multiply the number of tiles along each dimension OF ONE CHANNEL by the number of channels in each dimension to get the dimensionality of the full tile structure. */ tl->numtiles = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "tl->numtiles"); for(i=0;inumtiles[i] = tl->numtilesinch[i] * tl->numchannels[i]; tl->tottiles = gal_dimension_total_size(ndim, tl->numtiles); } /* Usage ----- Make a permutation to allow the conversion of tile location in memory to its location in the full input dataset and put it in the input's `permutation' element. If a permutation has already been defined for the tessellation, this function will not do anythin. If permutation won't be necessary, then this function will just return (the permutation must have been initialized to NULL). */ void gal_tile_full_permutation(struct gal_tile_two_layer_params *tl) { size_t *ch_coord, *tinch_coord; size_t i, p=0, t, ch, ind_in_all, ndim=tl->ndim; /* If the permutation has already been defined for this tessellation, then there is no need to do it again here. */ if(tl->permutation) return; /* If there is only one channel or one dimension, return NULL. The permutation functions know that the input and output indexs are the same when the permutation is NULL. */ if( ndim==1 || tl->totchannels==1) return; /* Allocate the space for the permutation and coordinates. */ ch_coord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "ch_coord"); tinch_coord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "tinch_coord"); tl->permutation=gal_data_malloc_array(GAL_TYPE_SIZE_T, tl->tottiles, __func__, "tl->permutation"); /* Fill in the permutation, we use the fact that the tiles are filled from the first channel to the last. */ for(ch=0;chtotchannels;++ch) { /* Get the coordinates of this channel's first tile. */ gal_dimension_index_to_coord(ch, ndim, tl->numchannels, ch_coord); for(i=0;inumtilesinch[i]; /* Go over all the tiles in this channel. */ for(t=0;ttottilesinch;++t) { /* Convert its index to coordinates and add them to the channel's starting coordinates. */ gal_dimension_index_to_coord(t, ndim, tl->numtilesinch, tinch_coord); for(i=0;inumtiles, tinch_coord); tl->permutation[ind_in_all] = p++; } } /* Clean up and return. */ free(tinch_coord); free(ch_coord); } /* Write one value for each tile into a file. IMPORTANT: it is assumed that the values are in the same order as the tiles. tile[i] --> tilevalues[i] */ void gal_tile_full_values_write(gal_data_t *tilevalues, struct gal_tile_two_layer_params *tl, int withblank, char *filename, gal_fits_list_key_t *keys, char *program_string) { gal_data_t *disp; /* Make the dataset to be displayed. */ if(tl->oneelempertile) { if(tl->ndim>1 && tl->totchannels>1) { /* A small sanity check. */ if(tl->permutation==NULL) error(EXIT_FAILURE, 0, "%s: no permutation defined for the input " "tessellation", __func__); /* Writing tile values to disk is not done for checking, not for efficiency. So to be safe (allow the caller to work on multiple threads), we will copy the tile values, then permute those. */ disp = gal_data_copy(tilevalues); gal_permutation_apply(disp, tl->permutation); } else disp = tilevalues; } else disp=gal_tile_block_write_const_value(tilevalues, tl->tiles, withblank, 0); /* Write the array as a file and then clean up (if necessary). */ gal_fits_img_write(disp, filename, keys, program_string); if(disp!=tilevalues) gal_data_free(disp); } /* Smooth the given values with a flat kernel of the given width. */ gal_data_t * gal_tile_full_values_smooth(gal_data_t *tilevalues, struct gal_tile_two_layer_params *tl, size_t width, size_t numthreads) { size_t *kdsize, knum, i; gal_data_t *kernel, *smoothed; struct gal_tile_two_layer_params ttl={0}; int permute=tl->ndim>1 && tl->totchannels>1; /* Check if the width is odd. */ if(width%2==0) error(EXIT_FAILURE, 0, "%s: %zu not acceptable as width. It has to be " "an odd number", __func__, width); /* Prepare the kernel size along every dimension. */ kdsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, tl->ndim, __func__, "kdsize"); for(i=0;indim;++i) kdsize[i]=width; /* Make the kernel. */ kernel=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, tilevalues->ndim, kdsize, NULL, 0, -1, NULL, NULL, NULL); knum=gal_dimension_total_size(tl->ndim, kernel->dsize); for(i=0;iarray))[i]=1/((double)knum); /* Permute (if necessary). */ if(permute) { gal_tile_full_permutation(tl); gal_permutation_apply(tilevalues, tl->permutation); } /* Do the smoothing. */ if(tl->workoverch) smoothed=gal_convolve_spatial(tilevalues, kernel, numthreads, 1, 1); else { /* Create the tile structure. */ ttl.tilesize=tl->numtilesinch; ttl.numchannels=tl->numchannels; gal_tile_full_sanity_check("IMPOSSIBLE", "IMP_HDU", tilevalues, &ttl); gal_tile_full_two_layers(tilevalues, &ttl); /* Do the convolution separately on each channel. */ smoothed=gal_convolve_spatial(ttl.tiles, kernel, numthreads, 1, 0); /* Clean up. */ ttl.tilesize=ttl.numchannels=NULL; gal_tile_full_free_contents(&ttl); } /* Reverse the permutation. */ if(permute) gal_permutation_apply_inverse(smoothed, tl->permutation); /* Clean up and return; */ free(kdsize); gal_data_free(kernel); return smoothed; } size_t gal_tile_full_id_from_coord(struct gal_tile_two_layer_params *tl, size_t *coord) { /* This function only works for 10 dimensions. */ size_t i, tr, chid, tile[10]; /* Host channel's ID. */ for(i=0;indim;++i) tile[i] = tl->totchannels == 1 ? 0 : coord[i] / tl->channelsize[i]; chid=gal_dimension_coord_to_index(tl->ndim, tl->numchannels, tile); /* Find the tile within the channel. */ for(i=0;indim;++i) { tr=coord[i] % tl->channelsize[i]; if( tl->firsttsize[i] != tl->tilesize[i] ) tile[i] = ( tr <= tl->firsttsize[i] ? 0 : 1 + (tr - tl->firsttsize[i]) / tl->tilesize[i] ); else tile[i] = tr / tl->tilesize[i]; } /* Return the tile ID. */ return ( chid * tl->tottilesinch + gal_dimension_coord_to_index(tl->ndim, tl->numtilesinch, tile) ); } /* Clean up the allocated spaces in the parameters. */ void gal_tile_full_free_contents(struct gal_tile_two_layer_params *tl) { /* Free the simply allocated spaces. */ if(tl->tilesize) free(tl->tilesize); if(tl->numchannels) free(tl->numchannels); if(tl->channelsize) free(tl->channelsize); if(tl->numtiles) free(tl->numtiles); if(tl->numtilesinch) free(tl->numtilesinch); if(tl->tilecheckname) free(tl->tilecheckname); if(tl->permutation) free(tl->permutation); if(tl->firsttsize) free(tl->firsttsize); /* Free the arrays of `gal_data_t' for each tile and channel. */ if(tl->tiles) gal_data_array_free(tl->tiles, tl->tottiles, 0); if(tl->channels) gal_data_array_free(tl->channels, tl->totchannels, 0); } gnuastro-0.5/lib/threads.c0000644000175000017500000002625613121462410012512 00000000000000/********************************************************************* Functions to facilitate using threads. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* from Gnulib, in Gnuastro's source */ /*****************************************************************/ /********* Implementation of pthread_barrier ***************/ /*****************************************************************/ /* Re-implementation of the example code given in: http://blog.albertarmea.com/post/47089939939/using-pthread-barrier-on-mac-os-x */ #if GAL_CONFIG_HAVE_PTHREAD_BARRIER == 0 /* Initialize the barrier structure. A barrier is a high-level way to wait until several threads have finished. */ int pthread_barrier_init(pthread_barrier_t *b, pthread_barrierattr_t *attr, unsigned int limit) { int err; /* Sanity check: */ if(limit==0) { errno = EINVAL; error(EXIT_FAILURE, errno, "%s: limit is zero", __func__); } /* Initialize the mutex: */ err=pthread_mutex_init(&b->mutex, 0); if(err) error(EXIT_FAILURE, err, "%s: inializing mutex", __func__); /* Initialize the condition variable: */ err=pthread_cond_init(&b->cond, 0); if(err) { pthread_mutex_destroy(&b->mutex); error(EXIT_FAILURE, err, "%s: inializing cond", __func__); } /* set the values: */ b->limit=limit; b->condfinished=b->count=0; return 0; } /* Suspend the calling thread (tell it to wait), until the limiting number of barriers is reached by the other threads. When the number isn't reached yet (process goes into the `else'), then we use the `pthread_cond_wait' function, which will wait until a broadcast is announced by another thread that succeeds the `if'. After the thread no longer needs the condition variable, we increment `b->condfinished' so `pthread_barrier_destroy' can know if it should wait (sleep) or continue.*/ int pthread_barrier_wait(pthread_barrier_t *b) { pthread_mutex_lock(&b->mutex); ++b->count; if(b->count >= b->limit) { pthread_cond_broadcast(&b->cond); ++b->condfinished; pthread_mutex_unlock(&b->mutex); return 1; } else { /* Initially b->count is smaller than b->limit, otherwise control would never have reached here. However, when it get to `pthread_cond_wait', this thread goes into a suspended period and is only awaken when a broad-cast is made. But we only want this thread to finish when b->count >= b->limit, so we have this while loop. */ while(b->count < b->limit) pthread_cond_wait(&b->cond, &b->mutex); ++b->condfinished; pthread_mutex_unlock(&b->mutex); return 0; } } /* Wait until all the threads that were blocked behind this barrier have finished (don't need the mutex and condition variable anymore. Then destroy the two. After this function, you can safely re-use the pthread_barrier_t structure. */ int pthread_barrier_destroy(pthread_barrier_t *b) { struct timespec request, remaining; /* Wait until no more threads need the barrier. */ request.tv_sec=0; request.tv_nsec=GAL_THREADS_BARRIER_DESTROY_NANOSECS; while( b->condfinished < b->limit ) nanosleep(&request, &remaining); /* Destroy the condition variable and mutex */ pthread_cond_destroy(&b->cond); pthread_mutex_destroy(&b->mutex); return 0; } #endif /* GAL_CONFIG_HAVE_PTHREAD_BARRIER == 0 */ /*******************************************************************/ /************ Thread utilities **************/ /*******************************************************************/ size_t gal_threads_number() { return num_processors(NPROC_CURRENT); } /* We have `numactions` jobs and we want their indexs to be divided between `numthreads` CPU threads. This function will give each index to a thread such that the maximum difference between the number of images for each thread is 1. The results will be saved in a 2D array of `outthrdcols` columns and each row will finish with a (size_t) -1, which is larger than any possible index!. */ void gal_threads_dist_in_threads(size_t numactions, size_t numthreads, size_t **outthrds, size_t *outthrdcols) { size_t *sp, *fp; size_t i, *thrds, thrdcols; *outthrdcols = thrdcols = numactions/numthreads+2; errno=0; thrds=*outthrds=malloc(numthreads*thrdcols*sizeof *thrds); if(thrds==NULL) error(EXIT_FAILURE, errno, "%s: allocating thrds", __func__); /* Initialize all the elements to NONINDEX. */ fp=(sp=thrds)+numthreads*thrdcols; do *sp=GAL_BLANK_SIZE_T; while(++spparams); size_t i; for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { THE INDEX OF THE TARGET IS NOW AVAILABLE AS `tprm->indexs[i]'. YOU CAN USE IT IN WHAT EVER MANNER YOU LIKE ALONG WITH THE SET OF VARIABLES/ARRAYS in `prm'. } if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } --------- High-level function --------- int higher_level_function(float *array, size_t num_in_array, int value1) { double value2; struct my_params; size_t numthreads; my_params.value1=value1; my_params.value2=value2; my_params.arary=array; gal_threads_spin_off(run_on_thread, &my_params, num_in_array, numthreads); return 1; } For real world applications of this function, you can also inspect the Gnuastro source. There are also many cases in Gnuastro where we benefit from this function. Please run the following command from the top source directory of Gnuastro to see where: $ grep -r gal_threads_spin_off ./ */ void gal_threads_spin_off(void *(*worker)(void *), void *caller_params, size_t numactions, size_t numthreads) { int err; pthread_t t; /* All thread ids saved in this, not used. */ pthread_attr_t attr; pthread_barrier_t b; struct gal_threads_params *prm; size_t i, *indexs, thrdcols, numbarriers; /* If there are no actions, then just return. */ if(numactions==0) return; /* Sanity check. */ if(numthreads==0) error(EXIT_FAILURE, 0, "%s: the number of threads (`numthreads') " "cannot be zero", __func__); /* Allocate the array of parameters structure structures. */ errno=0; prm=malloc(numthreads*sizeof *prm); if(prm==NULL) { fprintf(stderr, "%zu bytes could not be allocated for prm.", numthreads*sizeof *prm); exit(EXIT_FAILURE); } /* Distribute the actions into the threads: */ gal_threads_dist_in_threads(numactions, numthreads, &indexs, &thrdcols); /* Do the job: when only one thread is necessary, there is no need to spin off one thread, just call the workerfunction directly (spinning off threads is expensive). This is for the generic thread spinner function, not this simple function where `numthreads' is a constant. */ if(numthreads==1) { prm[0].id=0; prm[0].b=NULL; prm[0].indexs=indexs; prm[0].params=caller_params; worker(&prm[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barriers should be one more than the number of threads spinned off. */ numbarriers = (numactions Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include /************************************************************************/ /*************** Error messages ***************/ /************************************************************************/ void gal_tableintern_error_col_selection(char *filename, char *hdu, char *errorstring) { char *c, *name, *command; /* Set the proper pointers. */ if(gal_fits_name_is_fits(filename)) { asprintf(&name, "%s (hdu: %s)", filename, hdu); c=hdu; while(*c!='\0') if(isspace(*c++)) break; asprintf(&command, *c=='\0' ? "%s --hdu=%s" : "%s --hdu=\"%s\"", filename, hdu); } else command=name=filename; /* Abort with with the proper error. */ error(EXIT_FAILURE, 0, "%s: %s\n\nFor more information on selecting " "columns in Gnuastro, please run the following command (press " "`SPACE' to go down and `q' to return to the command-line):\n\n" " $ info gnuastro \"Selecting table columns\"\n\n" "To define a better column selection criteria, you can see " "the list of column meta-data in this table, with the following " "command:\n\n" " $ asttable %s --info\n", name, errorstring, command); } /************************************************************************/ /*************** Formats ***************/ /************************************************************************/ /* Return the type of desired table based on a standard string. */ uint8_t gal_tableintern_string_to_format(char *string) { if(string) /* Its not NULL. */ { if(!strcmp(string, "txt")) return GAL_TABLE_FORMAT_TXT; else if(!strcmp(string,"fits-ascii")) return GAL_TABLE_FORMAT_AFITS; else if(!strcmp(string, "fits-binary")) return GAL_TABLE_FORMAT_BFITS; else return GAL_TABLE_FORMAT_INVALID; } else return GAL_TABLE_FORMAT_INVALID; } char * gal_tableintern_format_as_string(uint8_t tableformat) { switch(tableformat) { case GAL_TABLE_FORMAT_TXT: return "txt"; case GAL_TABLE_FORMAT_AFITS: return "fits-ascii"; case GAL_TABLE_FORMAT_BFITS: return "fits-binary"; default: error(EXIT_FAILURE, 0, "%s: code %d not recognized", __func__, tableformat); return NULL; } } /* In programs, the `searchin' variable is much more easier to format in as a description than an integer (which is what `gal_table_read_cols' needs). This function will check the string value and give the corresponding integer value.*/ uint8_t gal_tableintern_string_to_searchin(char *string) { if(string) /* Its not NULL. */ { if(!strcmp(string, "name")) return GAL_TABLE_SEARCH_NAME; else if(!strcmp(string, "unit")) return GAL_TABLE_SEARCH_UNIT; else if(!strcmp(string, "comment")) return GAL_TABLE_SEARCH_COMMENT; else return GAL_TABLE_SEARCH_INVALID; } else return GAL_TABLE_SEARCH_INVALID; } char * gal_tableintern_searchin_as_string(uint8_t searchin) { switch(searchin) { case GAL_TABLE_SEARCH_NAME: return "name"; case GAL_TABLE_SEARCH_UNIT: return "unit"; case GAL_TABLE_SEARCH_COMMENT: return "comment"; default: error(EXIT_FAILURE, 0, "%s: code %d not recognized as a valid search " "field", __func__, searchin); return NULL; } } /* For programs that output tables, the `--tableformat' option will be used to specify what format the output table should be in. When the output file is a FITS file, there are multiple formats, so to simplify the coding in each program, this function will do a sanity check on the value given to the `--tableformat' parameter. */ void gal_tableintern_check_fits_format(char *filename, int tableformat) { if( filename && gal_fits_name_is_fits(filename) ) { /* When `--tableformat' was not given. */ if(tableformat==GAL_TABLE_FORMAT_INVALID) error(EXIT_FAILURE, 0, "`%s' (output file) is a FITS file but the " "desired format of the FITS table has not been specified with " "the `--tableformat' option. For FITS tables, this option can " "take two values: `fits-ascii', or `fits-binary'", filename); /* When `--tableformat' didn't have the correct value. */ if( tableformat != GAL_TABLE_FORMAT_AFITS && tableformat != GAL_TABLE_FORMAT_BFITS ) error(EXIT_FAILURE, 0, "`%s' (output file) is a FITS file but " "is not a recognized FITS table format. For FITS tables, " "`--tableformat' can take two values: `fits-ascii', or " "`fits-binary'", filename); } } /************************************************************************/ /*************** Printing information ***************/ /************************************************************************/ /* Fill in/adjust the basic information necessary to print a column. This information can be used for printing a plain text file or for FITS ASCII tables. The `fmt' and `lng' should point to pre-allocated arrays. The best way is: `char fmt[2], lng[3];' in the same function calling this. The width and precision, which are also necessary for printing, are updated in the data structure's `disp_width' and `disp_precision' elements. */ void gal_tableintern_col_print_info(gal_data_t *col, int tableformat, char *fmt, char *lng) { size_t j; char **strarr; int maxstrlen, width=0, precision=0; /* First do a sanity check, so we can safly stop checking in the steps below. */ switch(tableformat) { case GAL_TABLE_FORMAT_TXT: case GAL_TABLE_FORMAT_AFITS: break; default: error(EXIT_FAILURE, 0, "%s: is only for plain text or FITS ASCII " "tables. The input `tableformat' code %d not recognized", __func__, tableformat); } /* Set the formats and widths based on the type of the column. Initialize the characters and blank pointer. The long prefix is not necessary for most types, so just initialize it once up here.*/ fmt[0]=fmt[1]=lng[0]=lng[1]=lng[2]='\0'; switch(col->type) { case GAL_TYPE_BIT: error(EXIT_FAILURE, 0, "%s: printing of bit types is currently " "not supported", __func__); break; case GAL_TYPE_STRING: /* Set the basic information. */ fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 's' : 'A'; /* Go through all the strings in the column and find the maximum length to use as printing. If the user asked for a larger width (through the data structure's disp_width element), then set that. */ maxstrlen=0; strarr=col->array; for(j=0;jsize;++j) maxstrlen = ( (int)strlen(strarr[j]) > maxstrlen ? (int)strlen(strarr[j]) : maxstrlen ); width = col->disp_width>maxstrlen ? col->disp_width : maxstrlen; break; case GAL_TYPE_UINT8: case GAL_TYPE_UINT16: case GAL_TYPE_UINT32: case GAL_TYPE_UINT64: /* For the FITS ASCII table, there is only one format for all integers. */ if(tableformat==GAL_TABLE_FORMAT_AFITS) fmt[0]='I'; else switch(col->disp_fmt) { case GAL_TABLE_DISPLAY_FMT_UDECIMAL: fmt[0]='u'; break; case GAL_TABLE_DISPLAY_FMT_OCTAL: fmt[0]='o'; break; case GAL_TABLE_DISPLAY_FMT_HEX: fmt[0]='X'; break; default: fmt[0]='u'; } /* If we have a long type, then make changes. */ if(col->type==GAL_TYPE_UINT64) { lng[0]='l'; width=( col->disp_width<=0 ? GAL_TABLE_DEF_WIDTH_LINT : col->disp_width ); } else width=( col->disp_width<=0 ? GAL_TABLE_DEF_WIDTH_INT : col->disp_width ); precision=( col->disp_precision<=0 ? GAL_TABLE_DEF_PRECISION_INT : col->disp_precision ); break; case GAL_TYPE_INT8: case GAL_TYPE_INT16: case GAL_TYPE_INT32: fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 'd' : 'I'; width = ( col->disp_width<=0 ? GAL_TABLE_DEF_WIDTH_INT : col->disp_width ); precision = ( col->disp_precision<=0 ? GAL_TABLE_DEF_PRECISION_INT : col->disp_precision ); break; case GAL_TYPE_INT64: lng[0] = 'l'; fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 'd' : 'I'; width=( col->disp_width<=0 ? GAL_TABLE_DEF_WIDTH_LINT : col->disp_width ); precision=( col->disp_precision<=0 ? GAL_TABLE_DEF_PRECISION_INT : col->disp_precision ); break; /* We need a default value (because in most cases, it won't be set. */ case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: /* Set the format. */ switch(col->disp_fmt) { case GAL_TABLE_DISPLAY_FMT_FLOAT: fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 'f' : 'F'; break; case GAL_TABLE_DISPLAY_FMT_EXP: fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 'e' : 'E'; break; case GAL_TABLE_DISPLAY_FMT_GENERAL: fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 'g' : 'E'; break; default: fmt[0] = tableformat==GAL_TABLE_FORMAT_TXT ? 'g' : 'E'; break; } /* Set the width and precision */ switch(col->type) { case GAL_TYPE_FLOAT32: width = ( col->disp_width<=0 ? GAL_TABLE_DEF_WIDTH_FLT : col->disp_width ); precision = ( col->disp_precision<=0 ? GAL_TABLE_DEF_PRECISION_FLT : col->disp_precision ); break; case GAL_TYPE_FLOAT64: width = ( col->disp_width<=0 ? GAL_TABLE_DEF_WIDTH_DBL : col->disp_width ); /* CFITSIO doesn't recognize the double precision defined here for ASCII FITS tables. */ precision = ( col->disp_precision<=0 ? ( tableformat==GAL_TABLE_FORMAT_TXT ? GAL_TABLE_DEF_PRECISION_DBL : GAL_TABLE_DEF_PRECISION_FLT ) : col->disp_precision ); break; } break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, col->type); } /* Write the final width and precision into the column's data structure. */ col->disp_width=width; col->disp_precision=precision; } /* Use the input `blank' string and the input column to put the blank value in the column's array. This function should later be generalized into a function to read a string into a given data type (see `gal_data_string_to_array_elem'). It is only here temporarily. */ void gal_tableintern_read_blank(gal_data_t *col, char *blank) { /* If there is nothing to use as blank, then don't continue, note that the column data structure was initialized to mean that there is no blank value. */ if(blank==NULL) return; /* Just for a sanity check, the ndim and array elements should be zero. */ if(col->ndim || col->array) error(EXIT_FAILURE, 0, "%s: the number of dimensions, and the " "`array' element of `col' must be zero", __func__); /* Read the blank value as the given type. If successful, then `gal_data_string_to_type' will return 0. In that case, we need to initialize the necessary paramters to read this data structure correctly. */ if( !gal_type_from_string((void **)(&col->array), blank, col->type) ) { col->dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, 1, __func__, "col->dsize"); col->dsize[0]=col->ndim=col->size=1; } } gnuastro-0.5/lib/table.c0000644000175000017500000004512513211616535012154 00000000000000/********************************************************************* table -- Functions for I/O on tables. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include /************************************************************************/ /*************** Information about a table ***************/ /************************************************************************/ /* Store the information of each column in a table (either as a text file or as a FITS table) into an array of data structures with `numcols' structures (one data structure for each column). The number of rows is stored in `numrows'. The type of the table (e.g., ascii text file, or FITS binary or ASCII table) will be put in `tableformat' (macros defined in `gnuastro/table.h'. Note that other than the character strings (column name, units and comments), nothing in the data structure(s) will be allocated by this function for the actual data (e.g., the `array' or `dsize' elements). */ gal_data_t * gal_table_info(char *filename, char *hdu, size_t *numcols, size_t *numrows, int *tableformat) { /* Get the table format and size (number of columns and rows). */ if(gal_fits_name_is_fits(filename)) return gal_fits_tab_info(filename, hdu, numcols, numrows, tableformat); else { *tableformat=GAL_TABLE_FORMAT_TXT; return gal_txt_table_info(filename, numcols, numrows); } /* Abort with an error if we get to this point. */ error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so we can fix " "the problem. Control must not have reached the end of this function", __func__, PACKAGE_BUGREPORT); return NULL; } void gal_table_print_info(gal_data_t *allcols, size_t numcols, size_t numrows) { size_t i; int Nw=3, nw=4, uw=5, tw=4; /* Initial width from label's width */ char *name, *unit, *comment; /* Set the widths to print the column information. The width for the column number can easily be identified from the logarithm of the number of columns. */ Nw=log10(numcols)+1; for(i=0;inw) nw=strlen(allcols[i].name); if(allcols[i].unit && strlen(allcols[i].unit)>uw) uw=strlen(allcols[i].unit); if(allcols[i].type && strlen(gal_type_name(allcols[i].type, 1))>tw) tw=strlen(gal_type_name(allcols[i].type, 1)); } /* We want one column space between the columns for readability, not the exact length, so increment all the numbers. */ Nw+=2; nw+=2; uw+=2; tw+=2; /* Print these column names. */ printf("%-*s%-*s%-*s%-*s%s\n", Nw, "---", nw, "----", uw, "-----", tw, "----", "-------"); printf("%-*s%-*s%-*s%-*s%s\n", Nw, "No.", nw, "Name", uw, "Units", tw, "Type", "Comment"); printf("%-*s%-*s%-*s%-*s%s\n", Nw, "---", nw, "----", uw, "-----", tw, "----", "-------"); /* For each column, print the information, then free them. */ for(i=0;iname; case GAL_TABLE_SEARCH_UNIT: return col->unit; case GAL_TABLE_SEARCH_COMMENT: return col->comment; default: error(EXIT_FAILURE, 0, "%s: the code %d to searchin was not " "recognized", __func__, searchin); } error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "address the problem. Control must not have reached the end of " "this function", __func__, PACKAGE_BUGREPORT); return NULL; } static gal_list_sizet_t * make_list_of_indexs(gal_list_str_t *cols, gal_data_t *allcols, size_t numcols, int searchin, int ignorecase, char *filename, char *hdu, size_t *colmatch) { long tlong; int regreturn; regex_t *regex; gal_list_str_t *tmp; gal_list_sizet_t *indexll=NULL; size_t i, nummatch, colcount=0, len; char *str, *strcheck, *tailptr, *errorstring; /* Go over the given columns. */ if(cols) for(tmp=cols; tmp!=NULL; tmp=tmp->next) { /* Counter for number of columns matched, and length of name. */ nummatch=0; len=strlen(tmp->v); /* REGULAR EXPRESSION: the first and last characters are `/'. */ if( tmp->v[0]=='/' && tmp->v[len-1]=='/' ) { /* Remove the slashes, note that we don't want to change `tmp->v' (because it should be freed later). So first we set the last character to `\0', then define a new string from the first element. */ tmp->v[len-1]='\0'; str = tmp->v + 1; /* Allocate the regex_t structure: */ errno=0; regex=malloc(sizeof *regex); if(regex==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for regex", __func__, sizeof *regex); /* First we have to "compile" the string into the regular expression, see the "POSIX Regular Expression Compilation" section of the GNU C Library. About the case of the string: the FITS standard says: "It is _strongly recommended_ that every field of the table be assigned a unique, case insensitive name with this keyword..." So the column names can be case-sensitive. Here, we don't care about the details of a match, the only important thing is a match, so we are using the REG_NOSUB flag.*/ regreturn=0; regreturn=regcomp(regex, str, ( ignorecase ? RE_SYNTAX_AWK | REG_ICASE : RE_SYNTAX_AWK ) ); if(regreturn) table_regexerrorexit(regreturn, regex, str); /* With the regex structure "compile"d you can go through all the column names. Just note that column names are not mandatory in the FITS standard, so some (or all) columns might not have names, if so `p->tname[i]' will be NULL. */ for(i=0;iv[len-1]='/'; } /* Not regular expression. */ else { tlong=strtol(tmp->v, &tailptr, 0); /* INTEGER: If the string is an integer, then tailptr should point to the null character. If it points to anything else, it shows that we are not dealing with an integer (usable as a column number). So floating point values are also not acceptable. Since it is possible for the users to give zero for the column number, we need to read the string as a number first, then check it here. */ if(*tailptr=='\0') { /* Make sure the number is larger than zero! */ if(tlong<=0) error(EXIT_FAILURE, 0, "%s: column numbers must be " "positive (not zero or negative). You have asked " "for column number %ld", __func__, tlong); /* Check if the given value is not larger than the number of columns in the input catalog (note that the user is counting from 1, not 0!) */ if(tlong>numcols) error(EXIT_FAILURE, 0, "%s: has %zu columns, but you " "have asked for column number %ld", gal_fits_name_save_as_string(filename, hdu), numcols, tlong); /* Everything seems to be fine, put this column number in the output column numbers linked list. Note that internally, the column numbers start from 0, not 1.*/ gal_list_sizet_add(&indexll, tlong-1); ++nummatch; } /* EXACT MATCH: */ else { /* Go through all the desired column information and add the column number when there is a match. */ for(i=0;iv, strcheck) : !strcmp(tmp->v, strcheck) ) ) { ++nummatch; gal_list_sizet_add(&indexll, i); } } } } /* If there was no match, then report an error. This can only happen for string matches, not column numbers, for numbers, the checks are done (and program is aborted) before this step. */ if(nummatch==0) { asprintf(&errorstring, "`%s' didn't match any of the column %ss.", tmp->v, gal_tableintern_searchin_as_string(searchin)); gal_tableintern_error_col_selection(filename, hdu, errorstring); } /* Keep the value of `nummatch' if the user requested it. */ if(colmatch) colmatch[colcount++]=nummatch; } /* cols==NULL */ else for(i=0;i Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /**************************************************************** ******** Simple statistics ******* ****************************************************************/ /* Return the number of non-blank elements in an array as a single element, uint64 type data structure. */ gal_data_t * gal_statistics_number(gal_data_t *input) { size_t dsize=1; uint64_t counter=0; gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_UINT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* If there is no blank values in the input, then the total number is just the size. */ if(gal_blank_present(input, 0)) /* `{}' necessary for `else'. */ { GAL_TILE_PARSE_OPERATE(input, NULL, 0, 1, {++counter;}); } else counter = input->size; /* Write the value into memory. */ *((uint64_t *)(out->array)) = counter; return out; } /* Return the minimum (non-blank) value of a dataset in the same type as the dataset. Note that a NaN (blank in floating point) will fail on any comparison. So when finding the minimum or maximum, when the blank value is NaN, we can safely assume there is no blank value at all. */ gal_data_t * gal_statistics_minimum(gal_data_t *input) { size_t dsize=1, n=0; gal_data_t *out=gal_data_alloc(NULL, gal_tile_block(input)->type, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Initialize the output with the maximum possible value. */ gal_type_max(out->type, out->array); /* Parse the full input. */ GAL_TILE_PARSE_OPERATE(input, out, 0, 0, {*o = *i < *o ? *i : *o; ++n;}); /* If there were no usable elements, set the output to blank, then return. */ if(n==0) gal_blank_write(out->array, out->type); return out; } /* Return the maximum (non-blank) value of a dataset in the same type as the dataset. See explanations of `gal_statistics_minimum'. */ gal_data_t * gal_statistics_maximum(gal_data_t *input) { size_t dsize=1, n=0; gal_data_t *out=gal_data_alloc(NULL, gal_tile_block(input)->type, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Initialize the output with the minimum possible value. */ gal_type_min(out->type, out->array); /* Parse the full input. */ GAL_TILE_PARSE_OPERATE(input, out, 0, 0, {*o = *i > *o ? *i : *o; ++n;}); /* If there were no usable elements, set the output to blank, then return. */ if(n==0) gal_blank_write(out->array, out->type); return out; } /* Return the sum of the input dataset as a single element dataset of type float64. */ gal_data_t * gal_statistics_sum(gal_data_t *input) { size_t dsize=1, n=0; gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Parse the dataset. Note that in `gal_data_alloc' we set the `clear' flag to 1, so it will be 0.0f. */ GAL_TILE_PARSE_OPERATE(input, out, 0, 1, {++n; *o += *i;}); /* If there were no usable elements, set the output to blank, then return. */ if(n==0) gal_blank_write(out->array, out->type); return out; } /* Return the mean of the input dataset as a float64 type single-element dataset. */ gal_data_t * gal_statistics_mean(gal_data_t *input) { size_t dsize=1, n=0; gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Parse the dataset. Note that in `gal_data_alloc' we set the `clear' flag to 1, so it will be 0.0f. */ GAL_TILE_PARSE_OPERATE(input, out, 0, 1, {++n; *o += *i;}); /* Above, we calculated the sum and number, so if there were any elements in the dataset (`n!=0'), divide the sum by the number, otherwise, put a blank value in the output. */ if(n) *((double *)(out->array)) /= n; else gal_blank_write(out->array, out->type); return out; } /* Return the standard deviation of the input dataset as a single element dataset of type float64. */ gal_data_t * gal_statistics_std(gal_data_t *input) { size_t dsize=1, n=0; double s=0.0f, s2=0.0f; gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Parse the input. */ GAL_TILE_PARSE_OPERATE(input, out, 0, 1, {++n; s += *i; s2 += *i * *i;}); /* Write the standard deviation into the output. */ *((double *)(out->array)) = n ? sqrt( (s2-s*s/n)/n ) : GAL_BLANK_FLOAT64; return out; } /* Return the mean and standard deviation of a dataset in one run in type float64. The output is a two element data structure, with the first value being the mean and the second value the standard deviation. */ gal_data_t * gal_statistics_mean_std(gal_data_t *input) { size_t dsize=2, n=0; double s=0.0f, s2=0.0f; gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Parse the input. */ GAL_TILE_PARSE_OPERATE(input, out, 0, 1, {++n; s += *i; s2 += *i * *i;}); /* Write in the output values and return. */ ((double *)(out->array))[0] = n ? s/n : GAL_BLANK_FLOAT64; ((double *)(out->array))[1] = n ? sqrt( (s2-s*s/n)/n ) : GAL_BLANK_FLOAT64; return out; } /* The input is a sorted array with no blank values, we want the median value to be put inside the already allocated space which is pointed to by `median'. It is in the same type as the input. */ #define MED_IN_SORTED(IT) { \ IT *a=sorted->array; \ *(IT *)median = n%2 ? a[n/2] : (a[n/2]+a[n/2-1])/2; \ } static void statistics_median_in_sorted_no_blank(gal_data_t *sorted, void *median) { size_t n=sorted->size; switch(sorted->type) { case GAL_TYPE_UINT8: MED_IN_SORTED( uint8_t ); break; case GAL_TYPE_INT8: MED_IN_SORTED( int8_t ); break; case GAL_TYPE_UINT16: MED_IN_SORTED( uint16_t ); break; case GAL_TYPE_INT16: MED_IN_SORTED( int16_t ); break; case GAL_TYPE_UINT32: MED_IN_SORTED( uint32_t ); break; case GAL_TYPE_INT32: MED_IN_SORTED( int32_t ); break; case GAL_TYPE_UINT64: MED_IN_SORTED( uint64_t ); break; case GAL_TYPE_INT64: MED_IN_SORTED( int64_t ); break; case GAL_TYPE_FLOAT32: MED_IN_SORTED( float ); break; case GAL_TYPE_FLOAT64: MED_IN_SORTED( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, sorted->type); } } /* Return the median value of the dataset in the same type as the input as a one element dataset. If the `inplace' flag is set, the input data structure will be modified: it will have no blank values and will be sorted (increasing). */ gal_data_t * gal_statistics_median(gal_data_t *input, int inplace) { size_t dsize=1; gal_data_t *nbs=gal_statistics_no_blank_sorted(input, inplace);; gal_data_t *out=gal_data_alloc(NULL, nbs->type, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Write the median. */ statistics_median_in_sorted_no_blank(nbs, out->array); /* Clean up (if necessary), then return the output */ if(nbs!=input) gal_data_free(nbs); return out; } /* For a given size, return the index (starting from zero) that is at the given quantile. */ size_t gal_statistics_quantile_index(size_t size, double quantile) { double floatindex; /* Some sanity checks. */ if(size==0) { error(0, 0, "%s: `size' is 0. The quantile is not defined for " "a zero-sized array\n", __func__); return GAL_BLANK_SIZE_T; } if(quantile<0.0f || quantile>1.0f) error(EXIT_FAILURE, 0, "%s: the input quantile should be between 0.0 " "and 1.0 (inclusive). You have asked for %g", __func__, quantile); /* Find the index of the quantile. */ floatindex=(double)(size-1)*quantile; /* printf("quantile: %f, size: %zu, findex: %f\n", quantile, size, floatindex); */ /* Note that in the conversion from float to size_t, the floor integer value of the float will be used. */ if( floatindex - (int)floatindex > 0.5 ) return floatindex+1; else return floatindex; } /* Return a single element dataset of the same type as input keeping the value that has the given quantile. */ gal_data_t * gal_statistics_quantile(gal_data_t *input, double quantile, int inplace) { void *blank; size_t dsize=1, index; gal_data_t *nbs=gal_statistics_no_blank_sorted(input, inplace); gal_data_t *out=gal_data_alloc(NULL, nbs->type, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Find the index of the quantile. */ index=gal_statistics_quantile_index(nbs->size, quantile); /* Write the value at this index into the output. */ if(index==GAL_BLANK_SIZE_T) { blank=gal_data_malloc_array(nbs->type, 1, __func__, "blank"); memcpy(out->array, blank, gal_type_sizeof(nbs->type)); free(blank); } else memcpy(out->array, gal_data_ptr_increment(nbs->array, index, nbs->type), gal_type_sizeof(nbs->type)); /* Clean up and return. */ if(nbs!=input) gal_data_free(nbs); return out; } /* Return the index of the (first) point in the sorted dataset that has the closest value to `value' (which has to be the same type as the `input' dataset). */ #define STATS_QFUNC(IT) { \ IT *r, *a=nbs->array, *af=a+nbs->size, v=*((IT *)(value->array)); \ \ /* For a reference. Since we are comparing with the previous. */ \ /* element, we need to start with the second element.*/ \ r=a++; \ \ /* Increasing array: */ \ if( *a < *(a+1) ) \ do if(*a>v) { if( v - *(a-1) < *a - v ) --a; break; } while(++atype!=value->type) error(EXIT_FAILURE, 0, "%s: the types of the input dataset and requested " "value have to be the same", __func__); /* Find the result: */ switch(nbs->type) { case GAL_TYPE_UINT8: STATS_QFUNC( uint8_t ); break; case GAL_TYPE_INT8: STATS_QFUNC( int8_t ); break; case GAL_TYPE_UINT16: STATS_QFUNC( uint16_t ); break; case GAL_TYPE_INT16: STATS_QFUNC( int16_t ); break; case GAL_TYPE_UINT32: STATS_QFUNC( uint32_t ); break; case GAL_TYPE_INT32: STATS_QFUNC( int32_t ); break; case GAL_TYPE_UINT64: STATS_QFUNC( uint64_t ); break; case GAL_TYPE_INT64: STATS_QFUNC( int64_t ); break; case GAL_TYPE_FLOAT32: STATS_QFUNC( float ); break; case GAL_TYPE_FLOAT64: STATS_QFUNC( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, nbs->type); } /* Clean up and return. */ if(nbs!=input) gal_data_free(nbs); return index; } /* Return the quantile function of the given value as float64. */ gal_data_t * gal_statistics_quantile_function(gal_data_t *input, gal_data_t *value, int inplace) { double *d; size_t dsize=1; gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); size_t ind=gal_statistics_quantile_function_index(input, value, inplace); /* Note that counting of the index starts from 0, so for the quantile we should divided by (size - 1). */ d=out->array; d[0] = ( ind==-1 ? NAN : ((double)ind) / ((double)(input->size - 1)) ); return out; } /*********************************************************************/ /***************** Mode ***********************/ /*********************************************************************/ /* Main structure to keep mode parameters. */ struct statistics_mode_params { gal_data_t *data; /* Sorted input dataset with no blank values. */ size_t lowi; /* Lower quantile of interval. */ size_t midi; /* Index of the mid-interval point. */ size_t midd; /* Maximum CDF distance at the middle point. */ size_t highi; /* Higher quantile of interval. */ float tolerance; /* Tolerance level to terminate search. */ size_t numcheck; /* Number of pixels after mode to check. */ size_t interval; /* Interval to check pixels. */ float mirrordist; /* Distance after mirror to check ( x STD). */ }; /* Macros for the mode finding algorithm. */ #define MODE_MIN_Q 0.01f /* Mode search lower interval quantile. */ #define MODE_MAX_Q 0.55f /* Mode search higher interval quantile. */ #define MODE_GOOD_LQ 0.02f /* Least acceptable mode quantile. */ #define MODE_SYM_LOW_Q 0.01f /* Lower quantile to get symmetricity. */ #define MODE_GOLDEN_RATIO 1.618034f /* Golden ratio: (1+sqrt(5))/2. */ #define MODE_TWO_TAKE_GR 0.38197f /* 2 - Golden ratio. */ #define MODE_MIRROR_ABOVE (size_t)(-1) /* Mirror is above the result. */ /* Given a mirror point (`m'), return the maximum distance between the mirror distribution and the original distribution. The basic idea behind finding the mode is comparing the mirrored CDF (where the mirror is a test for the mode) with the original CDF for a given point. The job of this function is to return the maximum distance, given a mirror point. It takes the index of the mirror that is to be checked, it then finds the maximum difference between the mirrored CDF about the given point and the input CDF. `zf` keeps the value at the mirror (zero) point. `i` is used to count the pixels after the mirror in the mirror distribution. So `m+i` is the index of the mirrored distribution and mf=zf+(zf-a[m-i])=2*zf-a[m-i] is the mirrored flux at this point. Having found `mf', we find the `j` such that a[m+j] has the nearest flux to `mf`. The desired difference between the input CDF and the mirrored one for each `i` is then simply: `j-i`. Once `i` is incremented, `mf` will increase, so to find the new `j` we don't need to begin looking from `j=0`. Remember that the array is sorted, so the desired `j` is definitely larger than the previous `j`. So, if we keep the previous `j` in `prevj` then, all we have to do is to start incrementing `j` from `prevj`. This will really help in speeding up the job :-D. Only for the first element, `prevj=0`. */ #define MIRR_MAX_DIFF(IT) { \ IT *a=p->data->array, zf=a[m], mf=2*zf-a[m-i]; \ \ /* When a[m+j]>mf, we have reached the last pixel to check. Now, */ \ /* we just have to see which one of a[m+j-1] or a[m+j] is closer */ \ /* to `mf'. We then change `j` accordingly and break out of the */ \ /* `j' loop. */ \ for(j=prevj;jmf) \ { \ if( a[m+j]-mf < mf-a[m+j-1] ) \ break; \ else \ { \ j--; \ break; \ } \ } \ } static size_t mode_mirror_max_index_diff(struct statistics_mode_params *p, size_t m) { /* The variables: i: Index on mirror distribution. j: Index on input distribution. prevj: Index of previously checked point in the actual array. mf: (in macro) Value that is approximately equal in both distributions. */ size_t i, j, absdiff, prevj=0, size=p->data->size; size_t maxdiff=0, errordiff=p->mirrordist*sqrt(m); /* printf("###############\n###############\n"); printf("### Mirror pixel: %zu (mirrordist: %f, sqrt(m): %f)\n", m, p->mirrordist, sqrt(m)); printf("###############\n###############\n"); */ /* Go over the mirrored points. */ for(i=1; inumcheck && i<=m && m+iinterval) { /* Find `j': the index of the closest point in the original distribution that has a value similar to the mirror distribution. */ switch(p->data->type) { case GAL_TYPE_UINT8: MIRR_MAX_DIFF( uint8_t ); break; case GAL_TYPE_INT8: MIRR_MAX_DIFF( int8_t ); break; case GAL_TYPE_UINT16: MIRR_MAX_DIFF( uint16_t ); break; case GAL_TYPE_INT16: MIRR_MAX_DIFF( int16_t ); break; case GAL_TYPE_UINT32: MIRR_MAX_DIFF( uint32_t ); break; case GAL_TYPE_INT32: MIRR_MAX_DIFF( int32_t ); break; case GAL_TYPE_UINT64: MIRR_MAX_DIFF( uint64_t ); break; case GAL_TYPE_INT64: MIRR_MAX_DIFF( int64_t ); break; case GAL_TYPE_FLOAT32: MIRR_MAX_DIFF( float ); break; case GAL_TYPE_FLOAT64: MIRR_MAX_DIFF( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, p->data->type); } /* printf("i:%-5zu j:%-5zu diff:%-5d maxdiff: %zu\n", i, j, (int)j-(int)i, maxdiff); */ /* The index of the actual CDF corresponding the the mirrored flux has been found. We want the mirrored distribution to be within the actual distribution, not beyond it, so the only acceptable results are when ij' are acceptable. So, only when `i>j+errordiff' the result is not acceptable! */ if(i>j+errordiff) { maxdiff = MODE_MIRROR_ABOVE; break; } absdiff = i>j ? i-j : j-i; if(absdiff>maxdiff) maxdiff=absdiff; prevj=j; } /* Return the maximum difference */ return maxdiff; } /* Find the mode through the Golden-section search. It is assumed that `mode_mirror_max_index_diff' has one minimum (within the statistical errors) in the function. To find that minimum, the golden section search algorithm is going to used. Read the Wikipedia article for a very nice introduction. In summary we will constantly be finding middle points in the given interval and thus decreasing the interval until a certain tolerance is reached. If the input interval is on points `a' and `b', then the middle point (lets call it `c', where c>a and chighi-p->midi > p->midi-p->lowi) di = p->midi + MODE_TWO_TAKE_GR * (float)(p->highi-p->midi); else di = p->midi - MODE_TWO_TAKE_GR * (float)(p->midi-p->lowi); /* Since these are all indexs (and positive) we don't need an absolute value, highi is also always larger than lowi! In some cases, the first (standard) condition might be satisfied, while highi-lowi<=2. In such cases, also jump out! */ if( (p->highi - p->lowi) < p->tolerance*(p->midi+di) || (p->highi - p->lowi) <= 3) return (p->highi+p->lowi)/2; /* Find the maximum difference for this mirror point. */ dd = mode_mirror_max_index_diff(p, di); /*------------------------------------------------------------------ { static int counter=1; char outname[500], command[1000]; char histsname[500], cfpsname[500]; sprintf(outname, "%dcmp.pdf", counter); sprintf(cfpsname, "%dcfps.txt", counter); sprintf(histsname, "%dhists.txt", counter); gal_mode_make_mirror_plots(p->sorted, p->size, di, histsname, cfpsname); sprintf(command, "./plot.py %s %s %s", histsname, cfpsname, outname); system(command); } -------------------------------------------------------------------*/ /* printf("lowi:%-5zu\tmidi:%-5zu(midd: %d)\thighi:%-5zu ----> " "dq: %-5zu di: %d\n", p->lowi, p->midi, (int)p->midd, p->highi, di, (int)dd); */ /* +++++++++++++ Start of addition to the golden section search. The mirrored distribution's cumulative frequency plot has be lower than the actual's cfp. If it isn't, `di` will be MODE_MIRROR_ABOVE. In this case, the normal golden section minimization is not going to give us what we want. So we have this modification. In such cases, we want the search to go to the lower interval. */ if(dd==MODE_MIRROR_ABOVE) { if( p->midi < di ) { p->highi=di; return mode_golden_section(p); } else { p->highi=p->midi; p->midi=di; p->midd=dd; return mode_golden_section(p); } } /* End of addition to the golden section search. +++++++++++++*/ /* This is the standard golden section search: */ if(ddmidd) { if(p->highi-p->midi > p->midi-p->lowi) { p->lowi = p->midi; p->midi = di; p->midd = dd; return mode_golden_section(p); } else { p->highi = p->midi; p->midi = di; p->midd = dd; return mode_golden_section(p); } } else { if(p->highi-p->midi > p->midi-p->lowi) { p->highi = di; return mode_golden_section(p); } else { p->lowi = di; return mode_golden_section(p); } } } /* Once the mode is found, we need to do a quality control. This quality control is the measure of its symmetricity. Let's assume the mode index is at `m', since an index is just a count, from the Poisson distribution, the error in `m' is sqrt(m). Now, let's take `b' to be the first point that the difference between the cumulative distribution of the mirror and actual data deviate more than sqrt(m). For a scale parameter, lets assume that the index of 5% of `m` is `a`. We could have taken the distribution minimum, but the scatter in the minimum can be too high! Now, the "symmetricity" of the mode can be defined as: (b-m)/(m-a). For a completly symmetric mode, this should be 1. Note that the search for `b` only goes to the 95% of the distribution. */ #define MODE_SYM(IT) { \ IT *a=p->data->array, af=0, bf=0, mf=0, fi; \ \ /* Set the values at the mirror and at `a' (see above). */ \ mf=a[m]; \ af=a[ gal_statistics_quantile_index(2*m+1, MODE_SYM_LOW_Q) ]; \ \ /* This loop is very similar to that of */ \ /* `mode_mirror_max_index_diff'. It will find the index where the */\ /* difference between the two cumulative frequency plots exceeds */ \ /* that of the error in the mirror index.*/ \ for(i=1; ifi) \ { \ if( a[m+j]-fi < fi-a[m+j-1] ) \ break; \ else \ { \ j--; \ break; \ } \ } \ \ if(i>j+errdiff || j>i+errdiff) \ { \ bi=m+i; \ break; \ } \ prevj=j; \ } \ \ /* bi==0 shows that no point with a larger difference could be */ \ /* found. So bi should be set to the end of the search region. */ \ if(bi==0) bi=topi; \ \ bf = *(IT *)b_val = a[bi]; \ /*printf("%zu: %f,%f,%f\n", m, (double)af, (double)mf, (double)bf);*/ \ \ /* For a bad result, return 0 (which will not output any mode). */ \ return bf==af ? 0 : (bf-mf)/(mf-af); \ } static double mode_symmetricity(struct statistics_mode_params *p, size_t m, void *b_val) { size_t i, j, bi=0, topi, errdiff, prevj=0, size=p->data->size; /* Set the basic constants. */ topi = 2*m>size-1 ? size-1 : 2*m; errdiff = p->mirrordist * sqrt(m); /* Do the process. */ switch(p->data->type) { case GAL_TYPE_UINT8: MODE_SYM( uint8_t ); break; case GAL_TYPE_INT8: MODE_SYM( int8_t ); break; case GAL_TYPE_UINT16: MODE_SYM( uint16_t ); break; case GAL_TYPE_INT16: MODE_SYM( int16_t ); break; case GAL_TYPE_UINT32: MODE_SYM( uint32_t ); break; case GAL_TYPE_INT32: MODE_SYM( int32_t ); break; case GAL_TYPE_UINT64: MODE_SYM( uint64_t ); break; case GAL_TYPE_INT64: MODE_SYM( int64_t ); break; case GAL_TYPE_FLOAT32: MODE_SYM( float ); break; case GAL_TYPE_FLOAT64: MODE_SYM( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, p->data->type); } /* Control shouldn't reach here! */ error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so we can " "address the problem. Control must not have reached the end of this " "function", __func__, PACKAGE_BUGREPORT); return NAN; } /* Return the mode and related parameters in a float64 `gal_data_t' with the following elements in its array, the array: array[0]: mode array[1]: mode quantile. array[2]: symmetricity. array[3]: value at the end of symmetricity. The inputs are: - `input' is the input dataset, it doesn't have to be sorted and can have blank values. - `mirrordist' is the maximum distance after the mirror point to check as a multiple of sigma. - `inplace' is either 0 or 1. If it is 1 and the input array has blank values and is not sorted, then the removal of blank values and sorting will occur in-place (input will be modified): all blank elements in the input array will be removed and it will be sorted. */ gal_data_t * gal_statistics_mode(gal_data_t *input, float mirrordist, int inplace) { double *oa; size_t modeindex; size_t dsize=4, mdsize=1; struct statistics_mode_params p; int type=gal_tile_block(input)->type; gal_data_t *tmptype=gal_data_alloc(NULL, type, 1, &mdsize, NULL, 1, -1, NULL, NULL, NULL); gal_data_t *b_val=gal_data_alloc(NULL, type, 1, &mdsize, NULL, 1, -1, NULL, NULL, NULL); gal_data_t *out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* A small sanity check. */ if(mirrordist<=0) error(EXIT_FAILURE, 0, "%s: %f not acceptable as a value to " "`mirrordist'. Only positive values can be given to it", __func__, mirrordist); /* Make sure the input doesn't have blank values and is sorted. */ p.data=gal_statistics_no_blank_sorted(input, inplace); /* It can happen that the whole array is blank. In such cases, `p.data->size==0', so set all output elements to NaN and return. */ oa=out->array; if(p.data->size==0) { oa[0]=oa[1]=oa[2]=oa[3]=NAN; return out; } /* Basic constants. */ p.tolerance = 0.01; p.mirrordist = mirrordist; p.numcheck = p.data->size/2; /* Fill in the interval: Checking every single element is over-kill, so if the dataset is large enough, we'll set an interval to only check elements at an interval (so only 1000 elements are checked). */ p.interval = p.numcheck>1000 ? p.numcheck/1000 : 1; /* Set the lower and higher acceptable indexes for the mode based on quantiles. */ p.lowi = gal_statistics_quantile_index(p.data->size, MODE_MIN_Q); p.highi = gal_statistics_quantile_index(p.data->size, MODE_MAX_Q); /* Having set the low and higher interval values, we will set the first middle point and also the maximum distance on that point. This is necessary to start the iteration. */ p.midi = ( ( (float)p.highi + MODE_GOLDEN_RATIO * (float)p.lowi ) / ( 1 + MODE_GOLDEN_RATIO ) ); p.midd = mode_mirror_max_index_diff(&p, p.midi); /* Do the golden-section search iteration, read the mode value from the input array and save it in the `tmptype' data structure that has the same type as the input. */ modeindex = mode_golden_section(&p); memcpy( tmptype->array, gal_data_ptr_increment(p.data->array, modeindex, p.data->type), gal_type_sizeof(p.data->type) ); /* Convert the mode (which is in the same type as the input at this stage) to float64. */ tmptype=gal_data_copy_to_new_type_free(tmptype, GAL_TYPE_FLOAT64); /* Put the first three values into the output structure. */ oa[0] = *((double *)(tmptype->array)); oa[1] = ((double)modeindex) / ((double)(p.data->size-1)); oa[2] = mode_symmetricity(&p, modeindex, b_val->array); /* If the symmetricity is good, put it in the output, otherwise set all output values to NaN. */ if(oa[2]>GAL_STATISTICS_MODE_GOOD_SYM) { b_val=gal_data_copy_to_new_type_free(b_val, GAL_TYPE_FLOAT64); oa[3] = *((double *)(b_val->array)); } else oa[0]=oa[1]=oa[2]=oa[3]=NAN; /* For a check: printf("mode: %g\nquantile: %g\nsymmetricity: %g\nsym value: %g\n", oa[0], oa[1], oa[2], oa[3]); */ /* Clean up (if necessary), then return the output */ if(p.data!=input) gal_data_free(p.data); gal_data_free(tmptype); gal_data_free(b_val); return out; } /* Make the mirror array. */ #define STATS_MKMIRROR(IT) { \ IT *a=noblank_sorted->array, *m=mirror->array; \ IT zf=a[index]; \ *mirror_val=zf; \ for(i=0;i<=index;++i) m[i] = a[i]; \ for(i=1;i<=index;++i) m[index+i] = 2 * zf - m[index - i]; \ } static gal_data_t * statistics_make_mirror(gal_data_t *noblank_sorted, size_t index, double *mirror_val) { size_t i, dsize = 2*index+1; gal_data_t *mirror=gal_data_alloc(NULL, noblank_sorted->type, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Make sure the index is less than or equal to the number of elements. */ if( index >= noblank_sorted->size ) error(EXIT_FAILURE, 0, "%s: the index value must be less than or equal " "to the number of elements in the input, but it isn't: index: " "%zu, size of input: %zu", __func__, index, noblank_sorted->size); /* Fill in the mirror array. */ switch(noblank_sorted->type) { case GAL_TYPE_UINT8: STATS_MKMIRROR( uint8_t ); break; case GAL_TYPE_INT8: STATS_MKMIRROR( int8_t ); break; case GAL_TYPE_UINT16: STATS_MKMIRROR( uint16_t ); break; case GAL_TYPE_INT16: STATS_MKMIRROR( int16_t ); break; case GAL_TYPE_UINT32: STATS_MKMIRROR( uint32_t ); break; case GAL_TYPE_INT32: STATS_MKMIRROR( int32_t ); break; case GAL_TYPE_UINT64: STATS_MKMIRROR( uint64_t ); break; case GAL_TYPE_INT64: STATS_MKMIRROR( int64_t ); break; case GAL_TYPE_FLOAT32: STATS_MKMIRROR( float ); break; case GAL_TYPE_FLOAT64: STATS_MKMIRROR( double ); break; } /* Return the mirrored distribution. */ return mirror; } /* Make a mirrored histogram and cumulative frequency plot with the mirror distribution of the input with a value at `value'. The output is a linked list of data structures: the first is the bins with one bin at the mirror point, the second is the histogram with a maximum of one and the third is the cumulative frequency plot. */ gal_data_t * gal_statistics_mode_mirror_plots(gal_data_t *input, gal_data_t *value, size_t numbins, int inplace, double *mirror_val) { gal_data_t *mirror, *bins, *hist, *cfp; gal_data_t *nbs=gal_statistics_no_blank_sorted(input, inplace); size_t ind=gal_statistics_quantile_function_index(nbs, value, inplace); /* If the given mirror was outside the range of the input, then index will be 0 (below the range) or -1 (above the range), in that case, we should return NULL. */ if(ind==-1 || ind==0) return NULL; /* Make the mirror array. */ mirror=statistics_make_mirror(nbs, ind, mirror_val); /* Set the bins for histogram and cdf. */ bins=gal_statistics_regular_bins(mirror, NULL, numbins, *mirror_val); /* Make the histogram: set it's maximum value to 1 for a nice comparison with the CDF. */ hist=gal_statistics_histogram(mirror, bins, 0, 1); /* Make the cumulative frequency plot. */ cfp=gal_statistics_cfp(mirror, bins, 1); /* Set the pointers to make a table and return. */ bins->next=hist; hist->next=cfp; return bins; } /**************************************************************** ******** Sort ******* ****************************************************************/ /* Check if the given dataset is sorted. Output values are: - 0: Dataset is not sorted. - 1: Dataset is sorted and increasing or equal. - 2: dataset is sorted and decreasing. */ #define IS_SORTED(IT) { \ IT *aa=input->array, *a=input->array, *af=a+input->size-1; \ if(a[1]>=a[0]) do if( *(a+1) < *a ) break; while(++a *a ) break; while(++a=aa[0] \ ? GAL_STATISTICS_SORTED_INCREASING \ : GAL_STATISTICS_SORTED_DECREASING ) \ : GAL_STATISTICS_SORTED_NOT ); \ } int gal_statistics_is_sorted(gal_data_t *input) { /* A one-element dataset can be considered, sorted, so we'll just return 1 (for sorted and increasing). */ if(input->size==1) return GAL_STATISTICS_SORTED_INCREASING; /* Do the check. */ switch(input->type) { case GAL_TYPE_UINT8: IS_SORTED( uint8_t ); break; case GAL_TYPE_INT8: IS_SORTED( int8_t ); break; case GAL_TYPE_UINT16: IS_SORTED( uint16_t ); break; case GAL_TYPE_INT16: IS_SORTED( int16_t ); break; case GAL_TYPE_UINT32: IS_SORTED( uint32_t ); break; case GAL_TYPE_INT32: IS_SORTED( int32_t ); break; case GAL_TYPE_UINT64: IS_SORTED( uint64_t ); break; case GAL_TYPE_INT64: IS_SORTED( int64_t ); break; case GAL_TYPE_FLOAT32: IS_SORTED( float ); break; case GAL_TYPE_FLOAT64: IS_SORTED( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, input->type); } /* Control shouldn't reach this point. */ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can fix the " "problem. Control must not have reached the end of this function", __func__, PACKAGE_BUGREPORT); return -1; } /* This function is ignorant to blank values, if you want to make sure there is no blank values, you can call `gal_blank_remove' first. */ #define STATISTICS_SORT(QSORT_F) { \ qsort(input->array, input->size, gal_type_sizeof(input->type), QSORT_F); \ } void gal_statistics_sort_increasing(gal_data_t *input) { switch(input->type) { case GAL_TYPE_UINT8: STATISTICS_SORT(gal_qsort_uint8_increasing); break; case GAL_TYPE_INT8: STATISTICS_SORT(gal_qsort_int8_increasing); break; case GAL_TYPE_UINT16: STATISTICS_SORT(gal_qsort_uint16_increasing); break; case GAL_TYPE_INT16: STATISTICS_SORT(gal_qsort_int16_increasing); break; case GAL_TYPE_UINT32: STATISTICS_SORT(gal_qsort_uint32_increasing); break; case GAL_TYPE_INT32: STATISTICS_SORT(gal_qsort_int32_increasing); break; case GAL_TYPE_UINT64: STATISTICS_SORT(gal_qsort_uint64_increasing); break; case GAL_TYPE_INT64: STATISTICS_SORT(gal_qsort_int64_increasing); break; case GAL_TYPE_FLOAT32: STATISTICS_SORT(gal_qsort_float32_increasing); break; case GAL_TYPE_FLOAT64: STATISTICS_SORT(gal_qsort_float64_increasing); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, input->type); } } /* See explanations above `gal_statistics_sort_increasing'. */ void gal_statistics_sort_decreasing(gal_data_t *input) { switch(input->type) { case GAL_TYPE_UINT8: STATISTICS_SORT(gal_qsort_uint8_decreasing); break; case GAL_TYPE_INT8: STATISTICS_SORT(gal_qsort_int8_decreasing); break; case GAL_TYPE_UINT16: STATISTICS_SORT(gal_qsort_uint16_decreasing); break; case GAL_TYPE_INT16: STATISTICS_SORT(gal_qsort_int16_decreasing); break; case GAL_TYPE_UINT32: STATISTICS_SORT(gal_qsort_uint32_decreasing); break; case GAL_TYPE_INT32: STATISTICS_SORT(gal_qsort_int32_decreasing); break; case GAL_TYPE_UINT64: STATISTICS_SORT(gal_qsort_uint64_decreasing); break; case GAL_TYPE_INT64: STATISTICS_SORT(gal_qsort_int64_decreasing); break; case GAL_TYPE_FLOAT32: STATISTICS_SORT(gal_qsort_float32_decreasing); break; case GAL_TYPE_FLOAT64: STATISTICS_SORT(gal_qsort_float64_decreasing); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, input->type); } } /* Return a dataset that has doesn't have blank values and is sorted. If the `inplace' value is set to 1, then the input array will be modified, otherwise, a new array will be allocated with the desired properties. So if it is already sorted and has blank values, the `inplace' variable is irrelevant. This function can also work on tiles, in that case, `inplace' is useless, because a tile doesn't own its dataset and the dataset is not contiguous. */ gal_data_t * gal_statistics_no_blank_sorted(gal_data_t *input, int inplace) { int sortstatus; gal_data_t *contig, *noblank, *sorted; /* If this is a tile, then first we have to copy it into a contiguous piece of memory. After this step, we will only be dealing with `contig' (for a contiguous patch of memory). */ if(input->block) { /* Copy the input into a contiguous patch of memory. */ contig=gal_data_copy(input); /* When the data was a tile, we have already copied the array into a separate allocated space. So to avoid any further copying, we will just set the `inplace' variable to 1. */ inplace=1; } else contig=input; /* Make sure there is no blanks in the array that will be used. After this step, we won't be dealing with `input' any more, but with `noblank'. */ if( gal_blank_present(contig, inplace) ) { /* See if we should allocate a new dataset to remove blanks or if we can use the actual contiguous patch of memory. */ noblank = inplace ? contig : gal_data_copy(contig); gal_blank_remove(noblank); /* If we are working in place, then mark that there are no blank pixels. */ if(inplace) { noblank->flag |= GAL_DATA_FLAG_BLANK_CH; noblank->flag &= ~GAL_DATA_FLAG_HASBLANK; } } else noblank=contig; /* Make sure the array is sorted. After this step, we won't be dealing with `noblank' any more but with `sorted'. */ sortstatus=gal_statistics_is_sorted(noblank); if( sortstatus ) { sorted=noblank; sorted->status=sortstatus; } else { if(inplace) sorted=noblank; else { if(noblank!=input) /* no-blank has already been allocated. */ sorted=noblank; else sorted=gal_data_copy(noblank); } gal_statistics_sort_increasing(sorted); sorted->status=GAL_STATISTICS_SORTED_INCREASING; } /* Return final array. */ return sorted; } /**************************************************************** ******** Histogram and Cumulative Frequency Plot ******* ****************************************************************/ /* Generate an array of regularly spaced elements. Input arguments: * The `input' set you want to apply the bins to. This is only necessary if the range argument is not complete, see below. If `range' has all the necessary information, you can pass a NULL pointer for `input'. * The `inrange' data structure keeps the desired range along each dimension of the input data structure, it has to be in float32 type. Note that if - If you want the full range of the dataset (in any dimensions, then just set `range' to NULL and the range will be specified from the minimum and maximum value of the dataset. - If there is one element for each dimension in range, then it is viewed as a quantile (Q), and the range will be: `Q to 1-Q'. - If there are two elements for each dimension in range, then they are assumed to be your desired minimum and maximum values. When either of the two are NaN, the minimum and maximum will be calculated for it. * The number of bins: must be larger than 0. * `onebinstart' A desired value for onebinstart. Note that with this option, the bins won't start and end exactly on the given range values, it will be slightly shifted to accommodate this request. The output is a 1D array (column) of type double, it has to be double to account for small differences on the bin edges. */ gal_data_t * gal_statistics_regular_bins(gal_data_t *input, gal_data_t *inrange, size_t numbins, double onebinstart) { size_t i; gal_data_t *bins, *tmp, *range; double *b, *ra, min=NAN, max=NAN, hbw, diff, binwidth; /* Some sanity checks. */ if(numbins==0) error(EXIT_FAILURE, 0, "%s: `numbins' cannot be given a value of 0", __func__); /* Set the minimum and maximum values. */ if(inrange && inrange->size) { /* Make sure we are dealing with a double type range. */ if(inrange->type==GAL_TYPE_FLOAT64) range=inrange; else range=gal_data_copy_to_new_type(inrange, GAL_TYPE_FLOAT64); /* Set the minimum and maximum of the bins. */ ra=range->array; if( (range->size)%2 ) error(EXIT_FAILURE, 0, "%s: quantile ranges are not implemented yet", __func__); else { /* If the minimum isn't set (is blank), find it. */ if( isnan(ra[0]) ) { tmp=gal_data_copy_to_new_type_free(gal_statistics_minimum(input), GAL_TYPE_FLOAT64); min=*((double *)(tmp->array)); gal_data_free(tmp); } else min=ra[0]; /* For the maximum, when it isn't set, we'll add a very small value, so all points are included. */ if( isnan(ra[1]) ) { tmp=gal_data_copy_to_new_type_free(gal_statistics_maximum(input), GAL_TYPE_FLOAT64); max=*((double *)(tmp->array))+1e-6; gal_data_free(tmp); } else max=ra[1]; } /* Clean up: if `range' was allocated. */ if(range!=inrange) gal_data_free(range); } /* No range was given, find the minimum and maximum. */ else { tmp=gal_data_copy_to_new_type_free(gal_statistics_minimum(input), GAL_TYPE_FLOAT64); min=*((double *)(tmp->array)); gal_data_free(tmp); tmp=gal_data_copy_to_new_type_free(gal_statistics_maximum(input), GAL_TYPE_FLOAT64); max=*((double *)(tmp->array)) + 1e-6; gal_data_free(tmp); } /* Allocate the space for the bins. */ bins=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &numbins, NULL, 0, input->minmapsize, "bin_center", input->unit, "Center value of each bin."); /* Set central bin values. */ b=bins->array; hbw = ( binwidth=(max-min)/numbins )/2; for(i=0;i onebinstart) break; if( i != numbins-1 ) { diff = onebinstart - (b[i]-hbw); for(i=0;istatus=GAL_STATISTICS_BINS_REGULAR; return bins; } /* Make a histogram of all the elements in the given dataset with bin values that are defined in the `inbins' structure (see `gal_statistics_regular_bins'). `inbins' is not mandatory, if you pass a NULL pointer, the bins structure will be built within this function based on the `numbins' input. As a result, when you have already defined the bins, `numbins' is not used. */ #define HISTOGRAM_TYPESET(IT) { \ IT *a=input->array, *af=a+input->size; \ do if( *a>=min && *astatus!=GAL_STATISTICS_BINS_REGULAR) error(EXIT_FAILURE, 0, "%s: the input bins are not regular. Currently " "it is only implemented for regular bins", __func__); /* Check if normalize and `maxone' are not called together. */ if(normalize && maxone) error(EXIT_FAILURE, 0, "%s: only one of `normalize' and `maxone' may " "be given", __func__); /* Allocate the histogram (note that we are clearning it so all values are zero. */ hist=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, bins->ndim, bins->dsize, NULL, 1, input->minmapsize, "hist_number", "counts", "Number of data points within each bin."); /* Set the minimum and maximum range of the histogram from the bins. */ d=bins->array; binwidth=d[1]-d[0]; max = d[bins->size - 1] + binwidth/2; min = d[0] - binwidth/2; /* Go through all the elements and find out which bin they belong to. */ h=hist->array; switch(input->type) { case GAL_TYPE_UINT8: HISTOGRAM_TYPESET(uint8_t); break; case GAL_TYPE_INT8: HISTOGRAM_TYPESET(int8_t); break; case GAL_TYPE_UINT16: HISTOGRAM_TYPESET(uint16_t); break; case GAL_TYPE_INT16: HISTOGRAM_TYPESET(int16_t); break; case GAL_TYPE_UINT32: HISTOGRAM_TYPESET(uint32_t); break; case GAL_TYPE_INT32: HISTOGRAM_TYPESET(int32_t); break; case GAL_TYPE_UINT64: HISTOGRAM_TYPESET(uint64_t); break; case GAL_TYPE_INT64: HISTOGRAM_TYPESET(int64_t); break; case GAL_TYPE_FLOAT32: HISTOGRAM_TYPESET(float); break; case GAL_TYPE_FLOAT64: HISTOGRAM_TYPESET(double); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, input->type); } /* For a check: { size_t i, *hh=hist->array; for(i=0;isize;++i) printf("%-10.4f%zu\n", f[i], hh[i]); } */ /* Find the reference to correct the histogram if necessary. */ if(normalize) { /* Set the reference. */ ref=0.0f; hist=gal_data_copy_to_new_type_free(hist, GAL_TYPE_FLOAT32); ff=(f=hist->array)+hist->size; do ref += *f++; while(fname); free(hist->unit); free(hist->comment); gal_checkset_allocate_copy("hist_normalized", &hist->name); gal_checkset_allocate_copy("frac", &hist->unit); gal_checkset_allocate_copy("Normalized histogram value for this bin.", &hist->comment); } if(maxone) { /* Calculate the reference. */ ref=-FLT_MAX; hist=gal_data_copy_to_new_type_free(hist, GAL_TYPE_FLOAT32); ff=(f=hist->array)+hist->size; do ref = *f>ref ? *f : ref; while(++fname); free(hist->unit); free(hist->comment); gal_checkset_allocate_copy("hist_maxone", &hist->name); gal_checkset_allocate_copy("frac", &hist->unit); gal_checkset_allocate_copy("Fractional histogram value for this bin " "when maximum bin value is 1.0.", &hist->comment); } /* Correct the histogram if necessary. */ if( !isnan(ref) ) { ff=(f=hist->array)+hist->size; do *f++ /= ref; while(fnext'. If `bin->next!=NULL', then it is assumed to be the histogram. If it is NULL, then the histogram will be calculated internally and freed after the job is finished. When a histogram is given and it is normalized, the CFP will also be normalized (even if the normalized flag is not set here): note that a normalized CFP's maximum value is 1. */ gal_data_t * gal_statistics_cfp(gal_data_t *input, gal_data_t *bins, int normalize) { double sum; float *f, *ff, *hf; gal_data_t *hist, *cfp; size_t *s, *sf, *hs, sums; /* Check if the bins are regular or not. For irregular bins, we can either use the old implementation, or GSL's histogram functionality. */ if(bins->status!=GAL_STATISTICS_BINS_REGULAR) error(EXIT_FAILURE, 0, "%s: the input bins are not regular. Currently " "it is only implemented for regular bins", __func__); /* Prepare the histogram. */ hist = ( bins->next ? bins->next : gal_statistics_histogram(input, bins, 0, 0) ); /* If the histogram has float32 type it was given by the user and is either normalized or its maximum was set to 1. We can only use it if it was normalized. If it isn't normalized, then we must ignore it and build the histogram here.*/ if(hist->type==GAL_TYPE_FLOAT32) { sum=0.0f; ff=(f=hist->array)+hist->size; do sum += *f++; while(ftype, bins->ndim, bins->dsize, NULL, 1, input->minmapsize, ( hist->type==GAL_TYPE_FLOAT32 ? "cfp_normalized" : "cfp_number" ), ( hist->type==GAL_TYPE_FLOAT32 ? "frac" : "count" ), ( hist->type==GAL_TYPE_FLOAT32 ? "Fraction of data elements from the start to this " "bin (inclusive)." : "Number of data elements from the start to this " "bin (inclusive).") ); /* Fill in the cumulative frequency plot. */ switch(hist->type) { case GAL_TYPE_SIZE_T: sums=0; hs=hist->array; sf=(s=cfp->array)+cfp->size; do sums = (*s += *hs++ + sums); while(++sarray; ff=(f=cfp->array)+cfp->size; do sum = (*f += *hf++ + sum); while(++ftype); } /* Normalize the CFP if the user asked for it and it wasn't normalized until now. */ if(normalize && cfp->type==GAL_TYPE_SIZE_T) { /* Find the sum, then divide the plot by it. Note that the sum must come from the histogram, not the CFP!*/ sums=0; cfp=gal_data_copy_to_new_type_free(cfp, GAL_TYPE_FLOAT32); sf=(s=hist->array)+hist->size; do sums += *s++; while(sarray)+cfp->size; do *f++ /= sums; while(fname); free(cfp->unit); free(cfp->comment); gal_checkset_allocate_copy("cfp_normalized", &cfp->name); gal_checkset_allocate_copy("frac", &cfp->unit); gal_checkset_allocate_copy("Fraction of data elements from the start " "to this bin (inclusive).", &cfp->comment); } /* If the histogram was allocated here, free it. */ if(hist!=bins->next) gal_data_free(hist); return cfp; } /**************************************************************** ***************** Outliers ******************** ****************************************************************/ /* Sigma-cilp a given distribution: Inputs: - `multip': multiple of the standard deviation, - `param' must be positive and determines the type of clipping: - param<1.0: interpretted as a tolerance level to stop clipping. - param>=1.0 and an integer: a specific number of times to do the clippping. Output elements (type FLOAT32): - 0: Number of points used. - 1: Median. - 2: Mean. - 3: Standard deviation. The way this function works is very simple: first it will sort the input (if it isn't sorted). Afterwards, it will recursively change the starting point of the array and its size, calcluating the basic statistics in each round to define the new starting point and size. */ #define SIGCLIP(IT) { \ IT *a = nbs->array, *af = a + nbs->size; \ IT *bf = nbs->array, *b = bf + nbs->size - 1; \ \ /* Remove all out-of-range elements from the start of the array. */ \ if(sortstatus==GAL_STATISTICS_SORTED_INCREASING) \ do if( *a > (*med - (multip * *std)) ) \ { start=a; break; } \ while(++a=bf); \ else \ do if( *b > (*med - (multip * *std)) ) \ { size=b-a+1; break; } \ while(--b>=bf); \ } gal_data_t * gal_statistics_sigma_clip(gal_data_t *input, float multip, float param, int inplace, int quiet) { void *start, *nbs_array; double *med, *mean, *std; uint8_t bytolerance = param>=1.0f ? 0 : 1; double oldmed=NAN, oldmean=NAN, oldstd=NAN; size_t num=0, one=1, four=4, size, oldsize; gal_data_t *median_i, *median_d, *out, *meanstd; int sortstatus, type=gal_tile_block(input)->type; gal_data_t *nbs=gal_statistics_no_blank_sorted(input, inplace); size_t maxnum = param>=1.0f ? param : GAL_STATISTICS_SIG_CLIP_MAX_CONVERGE; /* Some sanity checks. */ if( multip<=0 ) error(EXIT_FAILURE, 0, "%s: `multip', must be greater than zero. The " "given value was %g", __func__, multip); if( param<=0 ) error(EXIT_FAILURE, 0, "%s: `param', must be greater than zero. The " "given value was %g", __func__, param); if( param >= 1.0f && ceil(param) != param ) error(EXIT_FAILURE, 0, "%s: when `param' is larger than 1.0, it is " "interpretted as an absolute number of clips. So it must be an " "integer. However, your given value %g", __func__, param); /* Allocate the necessary spaces. */ out=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &four, NULL, 0, input->minmapsize, NULL, NULL, NULL); median_i=gal_data_alloc(NULL, type, 1, &one, NULL, 0, input->minmapsize, NULL, NULL, NULL); /* Print the comments. */ if(!quiet) printf("%-8s %-10s %-15s %-15s %-15s\n", "round", "number", "median", "mean", "STD"); /* Do the clipping, but first initialize the values that will be changed during the clipping: the start of the array and the array's size. */ size=nbs->size; sortstatus=nbs->status; nbs_array=start=nbs->array; while(numarray); median_d=gal_data_copy_to_new_type(median_i, GAL_TYPE_FLOAT64); /* Find the average and Standard deviation, note that both `start' and `size' will be different in the next round. */ nbs->array = start; nbs->size = oldsize = size; meanstd=gal_statistics_mean_std(nbs); /* Put the three final values in usable (with a type) pointers. */ med = median_d->array; mean = meanstd->array; std = &((double *)(meanstd->array))[1]; /* If the user wanted to view the steps, show it to them. */ if(!quiet) printf("%-8zu %-10zu %-15g %-15g %-15g\n", num+1, size, *med, *mean, *std); /* If we are to work by tolerance, then check if we should jump out of the loop. Normally, `oldstd' should be larger than std, because the possible outliers have been removed. If it is not, it means that we have clipped too much and must stop anyway, so we don't need an absolute value on the difference! */ if( bytolerance && num>0 && ((oldstd - *std) / *std) < param ) break; /* Clip all the elements outside of the desired range: since the array is sorted, this means to just change the starting pointer and size of the array. */ switch(type) { case GAL_TYPE_UINT8: SIGCLIP( uint8_t ); break; case GAL_TYPE_INT8: SIGCLIP( int8_t ); break; case GAL_TYPE_UINT16: SIGCLIP( uint16_t ); break; case GAL_TYPE_INT16: SIGCLIP( int16_t ); break; case GAL_TYPE_UINT32: SIGCLIP( uint32_t ); break; case GAL_TYPE_INT32: SIGCLIP( int32_t ); break; case GAL_TYPE_UINT64: SIGCLIP( uint64_t ); break; case GAL_TYPE_INT64: SIGCLIP( int64_t ); break; case GAL_TYPE_FLOAT32: SIGCLIP( float ); break; case GAL_TYPE_FLOAT64: SIGCLIP( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } /* Set the values from this round in the old elements, so the next round can compare with, and return then if necessary. */ oldmed = *med; oldstd = *std; oldmean = *mean; ++num; /* Clean up: */ gal_data_free(meanstd); gal_data_free(median_d); } /* If we were in tolerance mode and `num' and `maxnum' are equal (the loop didn't stop by tolerance), so the outputs should be NaN. */ out->status=num; if( bytolerance && num==maxnum ) { ((float *)(out->array))[0] = NAN; ((float *)(out->array))[1] = NAN; ((float *)(out->array))[2] = NAN; ((float *)(out->array))[3] = NAN; } else { ((float *)(out->array))[0] = size; ((float *)(out->array))[1] = oldmed; ((float *)(out->array))[2] = oldmean; ((float *)(out->array))[3] = oldstd; } /* Clean up and return. */ nbs->array=nbs_array; if(nbs!=input) gal_data_free(nbs); return out; } #if 0 /* Using the cumulative distribution function this funciton will remove outliers from a dataset. */ void gal_statistics_remove_outliers_flat_cdf(float *sorted, size_t *outsize) { printf("\n ... in gal_statistics_remove_outliers_flat_cdf ... \n"); exit(1); int firstfound=0; size_t size=*outsize, i, maxind; float *slopes, minslope, maxslope; /* Find a slopes array, think of the cumulative frequency plot when you want to think about slopes. */ errno=0; slopes=malloc(size*sizeof *slopes); if(slopes==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for slopes", __func__, size*sizeof *slopes); /* Calcuate the slope of the CDF and put it in the slopes array. */ for(i=1;i Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /************************************************************************/ /******************** Info **********************/ /************************************************************************/ size_t gal_dimension_total_size(size_t ndim, size_t *dsize) { size_t i, num=1; for(i=0;i1) for(i=ndim-2;i>=0;--i) out[i]=dsize[i+1]*out[i+1]; /* Return the allocated array. */ return out; } size_t gal_dimension_num_neighbors(size_t ndim) { if(ndim) return pow(3, ndim)-1; else error(EXIT_FAILURE, 0, "%s: ndim cannot be zero", __func__); return 0; } /************************************************************************/ /******************** Coordinates **********************/ /************************************************************************/ void gal_dimension_add_coords(size_t *c1, size_t *c2, size_t *out, size_t ndim) { size_t *end=c1+ndim; do *out++ = *c1++ + *c2++; while(c1 b[i]) ? (a[i]-b[i]) : (b[i]-a[i]); return out; } gnuastro-0.5/lib/qsort.c0000644000175000017500000000726313121462410012225 00000000000000/********************************************************************* forqsort -- Functions used by qsort to sort an array. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include /* Initialize the array for sorting indexs to NULL. */ float *gal_qsort_index_arr; int gal_qsort_index_float_decreasing(const void * a, const void * b) { float ta=gal_qsort_index_arr[ *(size_t *)a ]; float tb=gal_qsort_index_arr[ *(size_t *)b ]; return (tb > ta) - (tb < ta); } int gal_qsort_uint8_decreasing(const void *a, const void *b) { return ( *(uint8_t *)b - *(uint8_t *)a ); } int gal_qsort_uint8_increasing(const void *a, const void *b) { return ( *(uint8_t *)a - *(uint8_t *)b ); } int gal_qsort_int8_decreasing(const void *a, const void *b) { return ( *(int8_t *)b - *(int8_t *)a ); } int gal_qsort_int8_increasing(const void *a, const void *b) { return ( *(int8_t *)a - *(int8_t *)b ); } int gal_qsort_uint16_decreasing(const void *a, const void *b) { return ( *(uint16_t *)b - *(uint16_t *)a ); } int gal_qsort_uint16_increasing(const void *a, const void *b) { return ( *(uint16_t *)a - *(uint16_t *)b ); } int gal_qsort_int16_decreasing(const void *a, const void *b) { return ( *(int16_t *)b - *(int16_t *)a ); } int gal_qsort_int16_increasing(const void *a, const void *b) { return ( *(int16_t *)a - *(int16_t *)b ); } int gal_qsort_uint32_decreasing(const void *a, const void *b) { return ( *(uint32_t *)b - *(uint32_t *)a ); } int gal_qsort_uint32_increasing(const void *a, const void *b) { return ( *(uint32_t *)a - *(uint32_t *)b ); } int gal_qsort_int32_decreasing(const void *a, const void *b) { return ( *(int32_t *)b - *(int32_t *)a ); } int gal_qsort_int32_increasing(const void *a, const void *b) { return ( *(int32_t *)a - *(int32_t *)b ); } int gal_qsort_uint64_decreasing(const void *a, const void *b) { return ( *(uint64_t *)b - *(uint64_t *)a ); } int gal_qsort_uint64_increasing(const void *a, const void *b) { return ( *(uint64_t *)a - *(uint64_t *)b ); } int gal_qsort_int64_decreasing(const void *a, const void *b) { return ( *(int64_t *)b - *(int64_t *)a ); } int gal_qsort_int64_increasing(const void *a, const void *b) { return ( *(int64_t *)a - *(int64_t *)b ); } int gal_qsort_float32_decreasing(const void *a, const void *b) { float ta=*(float*)a; float tb=*(float*)b; return (tb > ta) - (tb < ta); } int gal_qsort_float32_increasing(const void *a, const void *b) { float ta=*(float*)a; float tb=*(float*)b; return (ta > tb) - (ta < tb); } int gal_qsort_float64_decreasing(const void *a, const void *b) { double ta=*(double*)a; double tb=*(double*)b; return (tb > ta) - (tb < ta); } int gal_qsort_float64_increasing(const void *a, const void *b) { double ta=*(double*)a; double tb=*(double*)b; return (ta > tb) - (ta < tb); } gnuastro-0.5/lib/polygon.c0000644000175000017500000003341213121462410012537 00000000000000/********************************************************************* Polygon related functions and macros. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /***************************************************************/ /************** MACROS ******************/ /***************************************************************/ /* The cross product of two points from the center. */ #define GAL_POLYGON_CROSS_PRODUCT(A, B) ( (A)[0]*(B)[1] - (B)[0]*(A)[1] ) /* Find the cross product (2*area) between three points. Each point is assumed to be a pointer that has atleast two values within it. */ #define GAL_POLYGON_TRI_CROSS_PRODUCT(A, B, C) \ ( ( (B)[0]-(A)[0] ) * ( (C)[1]-(A)[1] ) - \ ( (C)[0]-(A)[0] ) * ( (B)[1]-(A)[1] ) ) \ /* We have the line A-B. We want to see if C is to the left of this line or to its right. This function will return 1 if it is to the left. It uses the basic property of vector multiplication: If the three points are anti-clockwise (the point is to the left), then the vector multiplication is positive, if it is negative, then it is clockwise (c is to the right). Ofcourse it is very important that A be below or equal to B in both the X and Y directions. The rounding error might give -0.0000000000001 (I didn't count the number of zeros!!) instead of zero for the area. Zero would indicate that they are on the same line in this case this should give a true result. */ #define GAL_POLYGON_LEFT_OF_LINE(A, B, C) \ ( GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) > -GAL_POLYGON_ROUND_ERR ) /* >= 0 */ /* See if the three points are collinear, similar to GAL_POLYGON_LEFT_OF_LINE except that the result has to be exactly zero. */ #define GAL_POLYGON_COLLINEAR_WITH_LINE(A, B, C) \ (GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) > -GAL_POLYGON_ROUND_ERR \ && GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) < GAL_POLYGON_ROUND_ERR) /* == 0 */ /* Similar to GAL_POLYGON_LEFT_OF_LINE except that if they are on the same line, this will return 0 (so that it is not on the left). Therefore the name is "proper left". */ #define GAL_POLYGON_PROP_LEFT_OF_LINE(A, B, C) \ ( GAL_POLYGON_TRI_CROSS_PRODUCT((A), (B), (C)) > GAL_POLYGON_ROUND_ERR ) /* > 0 */ #define GAL_POLYGON_MIN_OF_TWO(A, B) ((A)<(B)+GAL_POLYGON_ROUND_ERR ? (A) : (B)) #define GAL_POLYGON_MAX_OF_TWO(A, B) ((A)>(B)-GAL_POLYGON_ROUND_ERR ? (A) : (B)) /***************************************************************/ /************** Basic operations ******************/ /***************************************************************/ /* Sort the pixels in anti clock-wise order.*/ void gal_polygon_ordered_corners(double *in, size_t n, size_t *ordinds) { double angles[GAL_POLYGON_MAX_CORNERS]; size_t i, tmp, aindexs[GAL_POLYGON_MAX_CORNERS], tindexs[GAL_POLYGON_MAX_CORNERS]; if(n>GAL_POLYGON_MAX_CORNERS) error(EXIT_FAILURE, 0, "%s: most probably a bug! The number of corners " "is more than %d. This is an internal value and cannot be set from " "the outside. Most probably some bug has caused this un-normal " "value. Please contact us at %s so we can solve this problem", __func__, GAL_POLYGON_MAX_CORNERS, PACKAGE_BUGREPORT); /* For a check: printf("\n\nBefore sorting:\n"); for(i=0;i in[ ordinds[1]*2 ]) { tmp=ordinds[0]; ordinds[0]=ordinds[1]; ordinds[1]=tmp; } /* We only have `n-1' more elements to sort, use the angle of the line between the three remaining points and the first point. */ for(i=0;i=GAL_POLYGON_MIN_OF_TWO(Aa[0], Ab[0])-GAL_POLYGON_ROUND_ERR && o[0]<=GAL_POLYGON_MAX_OF_TWO(Aa[0], Ab[0])+GAL_POLYGON_ROUND_ERR && o[1]>=GAL_POLYGON_MIN_OF_TWO(Aa[1], Ab[1])-GAL_POLYGON_ROUND_ERR && o[1]<=GAL_POLYGON_MAX_OF_TWO(Aa[1], Ab[1])+GAL_POLYGON_ROUND_ERR ) return 1; else return 0; } else return 0; } /* Clip (find the overlap of) two polygons. This function uses the Sutherland-Hodgman polygon clipping psudocode from Wikipedia: List outputList = subjectPolygon; for (Edge clipEdge in clipPolygon) do List inputList = outputList; outputList.clear(); Point S = inputList.last; for (Point E in inputList) do if (E inside clipEdge) then if (S not inside clipEdge) then outputList.add(ComputeIntersection(S,E,clipEdge)); end if outputList.add(E); else if (S inside clipEdge) then outputList.add(ComputeIntersection(S,E,clipEdge)); end if S = E; done done The difference is that we are not using lists, but arrays to keep polygon vertices. The two polygons are called Subject (`s') and Clip (`c') with `n' and `m' vertices respectively. The output is stored in `o' and the number of elements in the output are stored in what `*numcrn' (for number of corners) points to.*/ void gal_polygon_clip(double *s, size_t n, double *c, size_t m, double *o, size_t *numcrn) { double in[2*GAL_POLYGON_MAX_CORNERS], *S, *E; size_t t, ii=m-1, i=0, jj, j, outnum, innum; /* if(n>GAL_POLYGON_MAX_CORNERS || m>GAL_POLYGON_MAX_CORNERS) error(EXIT_FAILURE, 0, "the two polygons given to the function " "gal_polygon_clip in polygon.c have %zu and %zu vertices. They cannot" " have any values larger than %zu", n, m, GAL_POLYGON_MAX_CORNERS); */ /* 2*outnum because for each vertice, there are two elements. */ outnum=n; for(t=0;t<2*outnum;++t) o[t]=s[t]; while(i0) ++outnum; o[2*outnum]=E[0]; o[2*outnum+1]=E[1]; ++outnum; } else if( GAL_POLYGON_PROP_LEFT_OF_LINE(&c[ii*2], &c[i*2], S) ) if( seginfintersection(S, E, &c[ii*2], &c[i*2], &o[2*outnum])>0 ) ++outnum; /* { size_t k; printf("(%.3f, %.3f) -- (%.3f, %.3f): %zu\n", S[0], S[1], E[0], E[1], outnum); for(k=0;k Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include /*********************************************************************/ /*************** Permutation info *******************/ /*********************************************************************/ void gal_permutation_check(size_t *permutation, size_t size) { size_t i; for(i=0; iarray; /* If permutation is NULL, then it is assumed that the data doesn't need to be re-ordered. */ if(permutation) { /* Necessary initializations. */ width=gal_type_sizeof(input->type); tmp=gal_data_malloc_array(input->type, 1, __func__, "tmp"); /* Do the permutation. */ for(i=0;isize;++i) { k=permutation[i]; while(k>i) k=permutation[k]; if(k>=i) { pk = permutation[k]; if( pk != i ) { memcpy(tmp, &array[i*width], width); while(pk!=i) { memcpy(&array[k*width], &array[pk*width], width); k = pk; pk = permutation[k]; } memcpy(&array[k*width], tmp, width); } } } /* Clean up. */ free(tmp); } } /* Apply the inverse of given permutation on the input dataset, see `gal_permutation_apply_inverse'. */ void gal_permutation_apply_inverse(gal_data_t *input, size_t *permutation) { void *tmp, *ttmp; size_t i, k, pk, width; uint8_t *array=input->array; if(permutation) { /* Initializations */ width=gal_type_sizeof(input->type); tmp=gal_data_malloc_array(input->type, 1, __func__, "tmp"); ttmp=gal_data_malloc_array(input->type, 1, __func__, "ttmp"); /* Re-order the values. */ for(i=0;isize;++i) { k=permutation[i]; while(k>i) k=permutation[k]; if(k>=i) { pk = permutation[k]; if(pk!=i) { memcpy(tmp, &array[k*width], width); while(pk!=i) { memcpy(ttmp, &array[pk*width], width); memcpy(&array[pk*width], tmp, width); memcpy(tmp, ttmp, width); k = pk; pk = permutation[k]; } memcpy(&array[pk*width], tmp, width); } } } /* Clean up. */ free(tmp); free(ttmp); } } gnuastro-0.5/lib/options.c0000644000175000017500000021006013216276304012551 00000000000000/********************************************************************* Function to parse options and configuration file values. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /**********************************************************************/ /************ Option utilities ***************/ /**********************************************************************/ int gal_options_is_last(struct argp_option *option) { return ( option->key==0 && option->name==NULL && option->doc==NULL && option->group==0 ); } int gal_options_is_category_title(struct argp_option *option) { return ( option->key==0 && option->name==NULL ); } void gal_options_add_to_not_given(struct gal_options_common_params *cp, struct argp_option *option) { gal_list_str_add(&cp->novalue_doc, (char *)option->doc, 0); gal_list_str_add(&cp->novalue_name, (char *)option->name, 0); } void gal_options_abort_if_mandatory_missing(struct gal_options_common_params *cp) { int namewidth=0; gal_list_str_t *tmp; char info[5000], *name, *doc; /* If there is no mandatory options, then just return. */ if(cp->novalue_name==NULL) return; /* Get the maximum width of the given names: */ for(tmp=cp->novalue_name; tmp!=NULL; tmp=tmp->next) if( strlen(tmp->v) > namewidth ) namewidth=strlen(tmp->v); /* Print the introductory information. */ sprintf(info, "to continue, the following options need a value "); sprintf(info+strlen(info), "(parenthesis after option name contain its " "description):\n\n"); /* Print the list of options along with their description. */ while(cp->novalue_name!=NULL) { doc = gal_list_str_pop(&cp->novalue_doc); name = gal_list_str_pop(&cp->novalue_name); sprintf(info+strlen(info), " %-*s (%s\b)\n", namewidth+4, name, doc); } sprintf(info+strlen(info), "\n"); /* Print suggestions, way to solve it. */ sprintf(info+strlen(info), "Use the command-line or a configuration file " "to set value(s).\n\nFor a complete description of command-line " "options and configuration files, please see the \"Options\" and " "\"Configuration files\" section of the Gnuastro book " "respectively. You can read them on the command-line by running " "the following commands (type `SPACE' to flip through pages, type " "`Q' to return to the command-line):\n\n" " info gnuastro Options\n" " info gnuastro \"Configuration files\"\n"); error(EXIT_FAILURE, 0, "%s", info); } static char * options_get_home() { char *home; home=getenv("HOME"); if(home==NULL) error(EXIT_FAILURE, 0, "HOME environment variable not defined"); return home; } /**********************************************************************/ /************ Parser functions for common options ***************/ /**********************************************************************/ void * gal_options_check_version(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { /* Check if the given value is different from this version. */ if( strcmp(arg, PACKAGE_VERSION) ) { /* Print an error message and abort. */ error_at_line(EXIT_FAILURE, 0, filename, lineno, "version mis-match: " "you are running GNU Astronomy Utilities (Gnuastro) " "version `%s'. However, the `onlyversion' option is set " "to version `%s'.\n\n" "This was probably done for reproducibility. Therefore, " "manually removing, or changing, the option value might " "produce errors or unexpected results. It is thus " "strongly advised to build Gnuastro %s and re-run this " "command/script.\n\n" "You can download previously released tar-balls from the " "following URLs respectively:\n\n" " Stable (version format: X.Y): " "http://ftpmirror.gnu.org/gnuastro\n" " Alpha (version format: X.Y.A-B): " "http://alpha.gnu.org/gnu/gnuastro\n\n" "Alternatively, you can clone Gnuastro, checkout the " "respective commit (from the version number), then " "bootstrap and build it. Please run the following " "command for more information:\n\n" " $ info gnuastro \"Version controlled source\"\n", PACKAGE_VERSION, arg, arg); /* Just to avoid compiler warnings for unused variables. The program will never reach this point! */ arg=filename=NULL; lineno=0; option=NULL; junk=NULL; } return NULL; } void * gal_options_print_citation(struct argp_option *option, char *arg, char *filename, size_t lineno, void *pa) { struct gal_options_common_params *cp=(struct gal_options_common_params *)pa; char *gnuastro_acknowledgement; char *gnuastro_bibtex= "Gnuastro package/infrastructure\n" "-------------------------------\n" " @ARTICLE{2015ApJS..220....1A,\n" " author = {{Akhlaghi}, M. and {Ichikawa}, T.},\n" " title = \"{Noise-based Detection and Segmentation of Nebulous " "Objects}\",\n" " journal = {\\apjs},\n" " archivePrefix = \"arXiv\",\n" " eprint = {1505.01664},\n" " primaryClass = \"astro-ph.IM\",\n" " keywords = {galaxies: irregular, galaxies: photometry, " "galaxies: structure, methods: data analysis, " "techniques: image processing, techniques: photometric},\n" " year = 2015,\n" " month = sep,\n" " volume = 220,\n" " eid = {1},\n" " pages = {1},\n" " doi = {10.1088/0067-0049/220/1/1},\n" " adsurl = {http://adsabs.harvard.edu/abs/2015ApJS..220....1A},\n" " adsnote = {Provided by the SAO/NASA Astrophysics Data System}\n" " }"; /* Print the statements. */ printf("\nThank you for using %s (%s) %s.\n\n", cp->program_name, PACKAGE_NAME, PACKAGE_VERSION); printf("Citations and acknowledgement are vital for the continued " "work on Gnuastro.\n\n" "Please cite the following record(s) and add the acknowledgement " "statement below in your work to support us. Please note that " "different Gnuastro programs may have different corresponding " "papers. Hence, please check all the programs you used. Don't " "forget to also include the version as shown above for " "reproducibility.\n\n" "%s\n\n", gnuastro_bibtex); /* Only print the citation for the program if one exists. */ if(cp->program_bibtex[0]!='\0') printf("%s\n\n", cp->program_bibtex); /* Notice for acknowledgements. */ asprintf(&gnuastro_acknowledgement, "Acknowledgement\n" "---------------\n" "This work was partly done using GNU Astronomy Utilities " "(Gnuastro) version %s. Gnuastro is a generic package for " "astronomical data manipulation and analysis which was " "initially created and developed for research funded by the " "Monbukagakusho (Japanese government) scholarship and ERC " "advanced grant 339659-MUSICOS.", PACKAGE_VERSION); printf("%s\n", gnuastro_acknowledgement); free(gnuastro_acknowledgement); /* Print a thank you message. */ printf(" ,\n" " {|'--.\n" " {{\\ \\\n" " Many thanks from all |/`'--./=.\n" " Gnuastro developers! `\\.---' `\\\\\n" " |\\ ||\n" " | |//\n" " \\//_/|\n" " //\\__/\n" " //\n" " (http://www.chris.com/ascii/) |/\n"); /* Exit the program. */ exit(EXIT_SUCCESS); /* Just to avoid compiler warnings for unused variables. The program will never reach this point! */ arg=filename=NULL; lineno=0; option=NULL; } void * gal_options_read_type(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { char *str; if(lineno==-1) { /* Note that `gal_data_type_as_string' returns a static string. But the output must be an allocated string so we can free it. */ gal_checkset_allocate_copy( gal_type_name( *(uint8_t *)(option->value), 1), &str); return str; } else { /* If the option is already set, just return. */ if(option->set) return NULL; /* Read the value. */ if ( (*(uint8_t *)(option->value) = gal_type_from_name(arg) ) == GAL_TYPE_INVALID ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' (value to " "`%s' option) couldn't be recognized as a known " "type.\n\nFor the full list of known types, please " "run the following command (press SPACE key to go " "down, and `q' to return to the command-line):\n\n" " $ info gnuastro \"Numeric data types\"\n", arg, option->name); /* For no un-used variable warning. This function doesn't need the pointer.*/ return junk=NULL; } } void * gal_options_read_searchin(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { char *str; if(lineno==-1) { /* Note that `gal_data_type_as_string' returns a static string. But the output must be an allocated string so we can free it. */ gal_checkset_allocate_copy( gal_tableintern_searchin_as_string( *(uint8_t *)(option->value)), &str); return str; } else { /* If the option is already set, just return. */ if(option->set) return NULL; /* Read the value. */ if((*(uint8_t *)(option->value)=gal_tableintern_string_to_searchin(arg)) == GAL_TABLE_SEARCH_INVALID ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' (value to " "`%s' option) couldn't be recognized as a known table " "search-in field (`name', `unit', or `comment').\n\n" "For more explanation, please run the following " "command (press SPACE key to go down, and `q' to " "return to the command-line):\n\n" " $ info gnuastro \"Selecting table columns\"\n", arg, option->name); /* For no un-used variable warning. This function doesn't need the pointer.*/ return junk=NULL; } } void * gal_options_read_tableformat(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { char *str; if(lineno==-1) { /* Note that `gal_data_type_as_string' returns a static string. But the output must be an allocated string so we can free it. */ gal_checkset_allocate_copy( gal_tableintern_format_as_string( *(uint8_t *)(option->value)), &str); return str; } else { /* If the option is already set, then you don't have to do anything. */ if(option->set) return NULL; /* Read the value. */ if( (*(uint8_t *)(option->value)=gal_tableintern_string_to_format(arg) ) ==GAL_TABLE_FORMAT_INVALID ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' (value to " "`%s' option) couldn't be recognized as a known table " "format field (`txt', `fits-ascii', or " "`fits-binary').\n\n", arg, option->name); /* For no un-used variable warning. This function doesn't need the pointer.*/ return junk=NULL; } } /* The input to this function is a string of any number of numbers separated by a comma (`,') and possibly containing fractions, for example: `1,2/3, 4.95'. The output `gal_data_t' contains the array of given values in `double' type. You can read the number from its `size' element. */ gal_data_t * gal_options_parse_list_of_numbers(char *string, char *filename, size_t lineno) { size_t i, num=0; gal_data_t *out; char *c=string, *tailptr; gal_list_f64_t *list=NULL, *tdll; double numerator=NAN, denominator=NAN, tmp; /* The nature of the arrays/numbers read here is very small, so since `p->cp.minmapsize' might not have been read yet, we will set it to -1 (largest size_t number), so the values are kept in memory. */ size_t minmapsize=-1; /* Go through the input character by character. */ while(string && *c!='\0') { switch(*c) { /* Ignore space or tab. */ case ' ': case '\t': ++c; break; /* Comma marks the transition to the next number. */ case ',': if(isnan(numerator)) error_at_line(EXIT_FAILURE, 0, filename, lineno, "a number " "must be given before `,'. You have given: `%s'", string); gal_list_f64_add(&list, isnan(denominator) ? numerator : numerator/denominator); numerator=denominator=NAN; ++num; ++c; break; /* Divide two numbers. */ case '/': if( isnan(numerator) || !isnan(denominator) ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`/' must " "only be between two numbers and used for " "division. But you have given `%s'", string); ++c; break; /* Extra dot is an error (cases like 2.5.5). Valid `.'s will be read by `strtod'. */ case '.': error_at_line(EXIT_FAILURE, 0, filename, lineno, "extra `.' in " "`%s'", string); break; /* Read the number. */ default: /* Parse the string. */ tmp=strtod(c, &tailptr); if(tailptr==c) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the first " "part of `%s' couldn't be read as a number. This " "was part of `%s'", c, string); /* See if the number should be put in the numerator or denominator. */ if(isnan(numerator)) numerator=tmp; else { if(isnan(denominator)) denominator=tmp; else error_at_line(EXIT_FAILURE, 0, filename, lineno, "more " "than two numbers in each element."); } /* Set `c' to tailptr. */ c=tailptr; } } /* If the last number wasn't finished by a `,', add the read value to the list */ if( !isnan(numerator) ) { ++num; gal_list_f64_add(&list, isnan(denominator) ? numerator : numerator/denominator); } /* Allocate the output data structure and fill it up. */ if(num) { i=num; out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &num, NULL, 0, minmapsize, NULL, NULL, NULL); for(tdll=list;tdll!=NULL;tdll=tdll->next) ((double *)(out->array))[--i]=tdll->v; } else { /* It is not possible to allocate a dataset with a size of 0 along any dimension (in C it's possible, but conceptually it isn't). So, we'll allocate space for one element, then free it. */ i=1; out=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &i, NULL, 0, minmapsize, NULL, NULL, NULL); out->size=out->dsize[0]=0; free(out->array); out->array=NULL; } /* Clean up and return. */ gal_list_f64_free(list); return out; } /* The input to this function is a string of any number of strings separated by a comma (`,') for example: `a,abc,abcd'. The output `gal_data_t' contains the array of given strings. You can read the number of inputs from its `size' element. */ gal_data_t * gal_options_parse_csv_strings_raw(char *string, char *filename, size_t lineno) { size_t i, num; gal_data_t *out; char *c=string, *str=NULL; gal_list_str_t *list=NULL, *tstrll=NULL; /* The nature of the arrays/numbers read here is very small, so since `p->cp.minmapsize' might not have been read yet, we will set it to -1 (largest size_t number), so the values are kept in memory. */ size_t minmapsize=-1; /* Go through the input character by character. */ while(string && *c!='\0') { switch(*c) { /* Comma marks the transition to the next string. */ case ',': if(str==NULL) error_at_line(EXIT_FAILURE, 0, filename, lineno, "a string " "must exist before the first `,'. You have " "given: `%s'", string); *c='\0'; gal_list_str_add(&list, str, 1); str=NULL; /* Mark that the next character is the start */ break; /* If the character isn't a coma, it is either in the middle of a string at the start of it. If `str==NULL', then it is at the start. */ default: if(str==NULL) str=c; } /* Increment C. */ ++c; } /* If the last element wasn't a comma, the last string hasn't been added to the list yet. */ if(str) gal_list_str_add(&list, str, 1); /* Allocate the output data structure and fill it up. */ if(list) { i=num=gal_list_str_number(list); out=gal_data_alloc(NULL, GAL_TYPE_STRING, 1, &num, NULL, 0, minmapsize, NULL, NULL, NULL); for(tstrll=list;tstrll!=NULL;tstrll=tstrll->next) ((char **)(out->array))[--i]=tstrll->v; } else { /* It is not possible to allocate a dataset with a size of 0 along any dimension (in C it's possible, but conceptually it isn't). So, we'll allocate space for one element, then free it. */ i=1; out=gal_data_alloc(NULL, GAL_TYPE_STRING, 1, &i, NULL, 0, minmapsize, NULL, NULL, NULL); out->size=out->dsize[0]=0; free(out->array); out->array=NULL; } /* Clean up and return. Note that we don't want to free the space of each string becuse it has been passed */ gal_list_str_free(list, 0); return out; } /* `arg' is the value given to an option. It contains multiple strings separated by a comma (`,'). This function will parse `arg' and make a `gal_data_t' array of strings from it. The output `gal_data_t' will be put in `option->value'. */ void * gal_options_parse_csv_strings(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { size_t nc; char *c, **strarr; int i, has_space=0; gal_data_t *values; char *str, sstr[GAL_OPTIONS_STATIC_MEM_FOR_VALUES]; /* We want to print the stored values. */ if(lineno==-1) { /* Set the pointer to the values dataset. */ values = *(gal_data_t **)(option->value); /* See if there are any space characters in the final string. */ strarr=values->array; for(i=0;isize;++i) if(has_space==0) { for(c=strarr[i];*c!='\0';++c) if(*c==' ' || *c=='\t') { has_space=1; break; } } /* If there is a space, the string must start wth quotation marks. */ nc = has_space ? 1 : 0; if(has_space) {sstr[0]='"'; sstr[1]='\0';} /* Write each string into the output string */ for(i=0;isize;++i) { if( nc > GAL_OPTIONS_STATIC_MEM_FOR_VALUES-100 ) error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so we " "can address the problem. The number of necessary " "characters in the statically allocated string has become " "too close to %d", __func__, PACKAGE_BUGREPORT, GAL_OPTIONS_STATIC_MEM_FOR_VALUES); nc += sprintf(sstr+nc, "%s,", strarr[i]); } /* If there was a space, we need a quotation mark at the end of the string. */ if(has_space) { sstr[nc-1]='"'; sstr[nc]='\0'; } else sstr[nc-1]='\0'; /* Copy the string into a dynamically allocated space, because it will be freed later.*/ gal_checkset_allocate_copy(sstr, &str); return str; } /* We want to read the user's string. */ else { /* If the option is already set, just return. */ if(option->set) return NULL; /* Read the values. */ values=gal_options_parse_csv_strings_raw(arg, filename, lineno); /* Put the values into the option. */ *(gal_data_t **)(option->value) = values; return NULL; } } /* Parse the given string into a series of size values (integers, stored as an array of size_t). The output array will be stored in the `value' element of the option. The last element of the array is `GAL_BLANK_SIZE_T' to allow finding the number of elements within it later (similar to a string which terminates with a '\0' element). */ void * gal_options_parse_sizes_reverse(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { int i; double *v; gal_data_t *values; size_t nc, num, *array; char *str, sstr[GAL_OPTIONS_STATIC_MEM_FOR_VALUES]; /* We want to print the stored values. */ if(lineno==-1) { /* Find the number of elements within the array. */ array = *(size_t **)(option->value); for(i=0; array[i]!=-1; ++i); num=i; /* Write all the dimensions into the static string. */ nc=0; for(i=num-1;i>=0;--i) { if( nc > GAL_OPTIONS_STATIC_MEM_FOR_VALUES-100 ) error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so we " "can address the problem. The number of necessary " "characters in the statically allocated string has become " "too close to %d", __func__, PACKAGE_BUGREPORT, GAL_OPTIONS_STATIC_MEM_FOR_VALUES); nc += sprintf(sstr+nc, "%zu,", array[i]); } sstr[nc-1]='\0'; /* Copy the string into a dynamically allocated space, because it will be freed later.*/ gal_checkset_allocate_copy(sstr, &str); return str; } /* We want to read the user's string. */ else { /* If the option is already set, just return. */ if(option->set) return NULL; /* Read the values. */ values=gal_options_parse_list_of_numbers(arg, filename, lineno); /* Check if the values are an integer. */ v=values->array; for(i=0;isize;++i) { if(v[i]<0) error_at_line(EXIT_FAILURE, 0, filename, lineno, "a given " "value in `%s' (%g) is not 0 or positive. The " "values to the `--%s' option must be positive", arg, v[i], option->name); if(ceil(v[i]) != v[i]) error_at_line(EXIT_FAILURE, 0, filename, lineno, "a given " "value in `%s' (%g) is not an integer. The " "values to the `--%s' option must be integers", arg, v[i], option->name); } /* Write the values into an allocated size_t array and finish it with a `-1' so the total number can be found later.*/ num=values->size; array=gal_data_malloc_array(GAL_TYPE_SIZE_T, num+1, __func__, "array"); for(i=0;ivalue) = array; gal_data_free(values); return NULL; } } /* Parse options with values of a list of numbers. */ void * gal_options_parse_csv_float64(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { size_t i, nc; double *darray; gal_data_t *values; char *str, sstr[GAL_OPTIONS_STATIC_MEM_FOR_VALUES]; /* We want to print the stored values. */ if(lineno==-1) { /* Set the pointer to the values dataset. */ values = *(gal_data_t **)(option->value); darray=values->array; /* Write each string into the output string */ nc=0; for(i=0;isize;++i) { if( nc > GAL_OPTIONS_STATIC_MEM_FOR_VALUES-100 ) error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so we " "can address the problem. The number of necessary " "characters in the statically allocated string has become " "too close to %d", __func__, PACKAGE_BUGREPORT, GAL_OPTIONS_STATIC_MEM_FOR_VALUES); nc += sprintf(sstr+nc, "%g,", darray[i]); } sstr[nc-1]='\0'; /* Copy the string into a dynamically allocated space, because it will be freed later.*/ gal_checkset_allocate_copy(sstr, &str); return str; } /* We want to read the user's string. */ else { /* If the option is already set, just return. */ if(option->set) return NULL; /* Read the values. */ values=gal_options_parse_list_of_numbers(arg, filename, lineno); /* Put the values into the option. */ *(gal_data_t **)(option->value) = values; /* The return value is only for printing mode, so we can return NULL after reading is complete. */ return NULL; } } /* Two numbers must be provided as an argument. This function will read them as the sigma-clipping multiple and parameter and store the two in a 2-element array. `option->value' must point to an already allocated 2-element array of double type. */ void * gal_options_read_sigma_clip(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { char *str; gal_data_t *in; double *sigmaclip=option->value; /* Caller wants to print the option values. */ if(lineno==-1) { asprintf(&str, "%g,%g", sigmaclip[0], sigmaclip[1]); return str; } /* Caller wants to read the values into memory, so parse the inputs. */ in=gal_options_parse_list_of_numbers(arg, filename, lineno); /* Check if there was only two numbers. */ if(in->size!=2) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the `--%s' " "option takes two values (separated by a comma) for " "defining the sigma-clip. However, %zu numbers were " "read in the string `%s' (value to this option).\n\n" "The first number is the multiple of sigma, and the " "second is either the tolerance (if its is less than " "1.0), or a specific number of times to clip (if it " "is equal or larger than 1.0).", option->name, in->size, arg); /* Copy the sigma clip parameters into the space the caller has given (as the `value' element of `option'). */ memcpy(option->value, in->array, 2*sizeof *sigmaclip); /* Multiple of sigma must be positive. */ if( sigmaclip[0] <= 0 ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the first value to " "the `--%s' option (multiple of sigma), must be " "greater than zero. From the string `%s' (value to " "this option), you have given a value of %g for the " "first value", option->name, arg, sigmaclip[0]); /* Second value must also be positive. */ if( sigmaclip[1] <= 0 ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the second value " "to the `--%s' option (tolerance to stop clipping or " "number of clips), must be greater than zero. From " "the string `%s' (value to this option), you have " "given a value of %g for the second value", option->name, arg, sigmaclip[1]); /* if the second value is larger or equal to 1.0, it must be an integer. */ if( sigmaclip[1] >= 1.0f && ceil(sigmaclip[1]) != sigmaclip[1]) error_at_line(EXIT_FAILURE, 0, filename, lineno, "when the second " "value to the `--%s' option is >=1, it is interpretted " "as an absolute number of clips. So it must be an " "integer. However, your second value is a floating " "point number: %g (parsed from `%s')", option->name, sigmaclip[1], arg); /* Clean up and return. */ gal_data_free(in); return NULL; } /**********************************************************************/ /************ Option actions ***************/ /**********************************************************************/ /* The option value has been read and put into the `value' field of the `argp_option' structure. This function will use the `range' field to define a check and abort with an error if the value is not in the given range. It also takes the `arg' so it can be used for good error message (showing the value that could not be read). */ static void options_sanity_check(struct argp_option *option, char *arg, char *filename, size_t lineno) { size_t dsize=1; char *message=NULL; int operator1=GAL_ARITHMETIC_OP_INVALID; int operator2=GAL_ARITHMETIC_OP_INVALID; int multicheckop=GAL_ARITHMETIC_OP_INVALID; gal_data_t *value, *ref1=NULL, *ref2=NULL, *check1, *check2; int mcflag = ( GAL_ARITHMETIC_NUMOK | GAL_ARITHMETIC_FREE | GAL_ARITHMETIC_INPLACE ); /* Currently, this function is only for numeric types, so if the value is string type, or its `range' field is `GAL_OPTIONS_RANGE_ANY', then just return without any checks. */ if( option->type==GAL_TYPE_STRING || option->type==GAL_TYPE_STRLL || option->range==GAL_OPTIONS_RANGE_ANY ) return; /* Put the option value into a data structure. */ value=gal_data_alloc(option->value, option->type, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); /* Set the operator(s) and operands: */ switch(option->range) { case GAL_OPTIONS_RANGE_GT_0: message="greater than zero"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; operator1=GAL_ARITHMETIC_OP_GT; ref2=NULL; break; case GAL_OPTIONS_RANGE_GE_0: message="greater or equal to zero"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; operator1=GAL_ARITHMETIC_OP_GE; ref2=NULL; break; case GAL_OPTIONS_RANGE_0_OR_1: message="either 0 or 1"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); ref2=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; *(unsigned char *)(ref2->array)=1; operator1=GAL_ARITHMETIC_OP_EQ; operator2=GAL_ARITHMETIC_OP_EQ; multicheckop=GAL_ARITHMETIC_OP_OR; break; case GAL_OPTIONS_RANGE_GE_0_LE_1: message="between zero and one (inclusive)"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); ref2=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; *(unsigned char *)(ref2->array)=1; operator1=GAL_ARITHMETIC_OP_GE; operator2=GAL_ARITHMETIC_OP_LE; multicheckop=GAL_ARITHMETIC_OP_AND; break; case GAL_OPTIONS_RANGE_GE_0_LT_1: message="between zero (inclusive) and one (exclusive)"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); ref2=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; *(unsigned char *)(ref2->array)=1; operator1=GAL_ARITHMETIC_OP_GE; operator2=GAL_ARITHMETIC_OP_LT; multicheckop=GAL_ARITHMETIC_OP_AND; break; case GAL_OPTIONS_RANGE_GT_0_LT_1: message="between zero and one (not inclusive)"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); ref2=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; *(unsigned char *)(ref2->array)=1; operator1=GAL_ARITHMETIC_OP_GT; operator2=GAL_ARITHMETIC_OP_LT; multicheckop=GAL_ARITHMETIC_OP_AND; break; case GAL_OPTIONS_RANGE_GT_0_ODD: message="greater than zero and odd"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); ref2=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; *(unsigned char *)(ref2->array)=2; operator1=GAL_ARITHMETIC_OP_GT; operator2=GAL_ARITHMETIC_OP_MODULO; multicheckop=GAL_ARITHMETIC_OP_AND; break; case GAL_OPTIONS_RANGE_0_OR_ODD: message="greater than, or equal to, zero and odd"; ref1=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); ref2=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); *(unsigned char *)(ref1->array)=0; *(unsigned char *)(ref2->array)=2; operator1=GAL_ARITHMETIC_OP_EQ; operator2=GAL_ARITHMETIC_OP_MODULO; multicheckop=GAL_ARITHMETIC_OP_OR; break; default: error(EXIT_FAILURE, 0, "%s: range code %d not recognized", __func__, option->range); } /* Use the arithmetic library to check for the condition. We don't want to free the value or change its value, so when dealing with the value directly, we won't use the `GAL_ARITHMETIC_FREE', or `GAL_ARITHMETIC_INPLACE' flags. But we will do this when there are multiple checks so from the two check data structures, we only have one remaining. */ check1=gal_arithmetic(operator1, GAL_ARITHMETIC_NUMOK, value, ref1); if(ref2) { check2=gal_arithmetic(operator2, GAL_ARITHMETIC_NUMOK, value, ref2); check1=gal_arithmetic(multicheckop, mcflag, check1, check2); } /* If the final check is not successful, then print an error. */ if( *(unsigned char *)(check1->array)==0 ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "value to option `%s' must be %s, but the given value " "is `%s'. Recall that `%s' is \"%s\"", option->name, message, arg, option->name, option->doc); /* Clean up and finish. Note that we used the actual value pointer in the data structure, so first we need to set it to NULL, so `gal_data_free' doesn't free it, we need it for later (for example to print the option values). */ value->array=NULL; gal_data_free(ref1); gal_data_free(ref2); gal_data_free(value); gal_data_free(check1); } static void gal_options_read_check(struct argp_option *option, char *arg, char *filename, size_t lineno, struct gal_options_common_params *cp) { void *topass; /* If a function is defined, leave everything to the function. */ if(option->func) { /* For the functions that are defined here (for all programs) and need the last pointer, we must pass the `cp' pointer. For the rest, we must pass the `cp->program_struct'. */ switch(option->key) { case GAL_OPTIONS_KEY_CITE: case GAL_OPTIONS_KEY_CONFIG: topass=cp; break; default: topass=cp->program_struct; } /* Call the function to parse the value, flag the option as set and return (except for the `--config' option, which must always be unset). */ option->func(option, arg, filename, lineno, topass); if(option->key!=GAL_OPTIONS_KEY_CONFIG) option->set=GAL_OPTIONS_SET; return; } /* Check if an argument is actually given (only options given on the command-line can have a NULL arg value). */ if(arg) { if(option->type==GAL_TYPE_STRLL) gal_list_str_add(option->value, arg, 1); else { /* If the option is already set, ignore the given value. */ if(option->set==GAL_OPTIONS_SET) return; /* Read the string argument into the value. */ if( gal_type_from_string(&option->value, arg, option->type) ) /* Fortunately `error_at_line' will behave like `error' when the filename is NULL (the option was read from a command-line). */ error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' (value to option `--%s') couldn't be read " "into the proper numerical type. Common causes " "for this error are:\n" " - It contains non-numerical characters.\n" " - It is negative, but the expected value is " "positive.\n" " - It is floating point, but the expected value " "is an integer.\n" " - The previous option required a value, but you " "forgot to give it one, so the next option's " "name(+value, if there are no spaces between them) " "is read as the value of the previous option.", arg, option->name); /* Do a sanity check on the value. */ options_sanity_check(option, arg, filename, lineno); } } else { /* If the option is already set, ignore the given value. */ if(option->set==GAL_OPTIONS_SET) return; /* Make sure the option has the type set for options with no argument. So, give it a value of 1. */ if(option->type==GAL_OPTIONS_NO_ARG_TYPE) *(uint8_t *)(option->value)=1; else error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " "correct it. Options with no arguments, must have " "type `%s'. However, the `%s' option has type %s", __func__, PACKAGE_BUGREPORT, gal_type_name(GAL_OPTIONS_NO_ARG_TYPE, 1), option->name, gal_type_name(option->type, 1)); } /* Flip the `set' flag to `GAL_OPTIONS_SET'. */ option->set=GAL_OPTIONS_SET; } /**********************************************************************/ /************ Command-line options ***************/ /**********************************************************************/ /* Set the value given to the command-line, where we have the integer `key' of the option, not its long name as a string. */ error_t gal_options_set_from_key(int key, char *arg, struct argp_option *options, struct gal_options_common_params *cp) { size_t i; /* Go through all the options and find the one that should keep this value, then put its value into the appropriate key. Note that the options array finishs with an all zero element, so we don't need to know the number before hand.*/ for(i=0;1;++i) { /* Check if the key corresponds to this option. */ if( options[i].key==key ) { /* When options are read from keys (by this function), they are read from the command-line. On the commandline, the last invokation of the option is important. Especially in contexts like scripts, this is important because you can change a given command-line option (that is not a linked list) by calling it a second time, instead of going back and changing the first value. As a result, only when searching for options on the command-line, a second value to the same option will replace the first one. This will not happen in configuration files. */ if(options[i].set && gal_type_is_list(options[i].type)==0) options[i].set=GAL_OPTIONS_NOT_SET; /* Parse the value. */ gal_options_read_check(&options[i], arg, NULL, 0, cp); /* We have found and set the value given to this option, so just return success (an error_t of 0 means success). */ return 0; } else { /* The last option has all its values set to zero. */ if(gal_options_is_last(&options[i])) return ARGP_ERR_UNKNOWN; } } } error_t gal_options_common_argp_parse(int key, char *arg, struct argp_state *state) { struct gal_options_common_params *cp=state->input; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Read the options. */ return gal_options_set_from_key(key, arg, cp->coptions, cp); } /**********************************************************************/ /************ Configuration files ***************/ /**********************************************************************/ /* Read the option and the argument from the line and return.*/ static void options_read_name_arg(char *line, char *filename, size_t lineno, char **name, char **arg) { int notyetfinished=1, inword=0, inquote=0; /* Initialize name and value: */ *arg=NULL; *name=NULL; /* Go through the characters and set the values: */ do switch(*line) { case ' ': case '\t': case '\v': case '\n': case '\r': if(inword) /* Only considered in a word, not in a quote*/ { inword=0; *line='\0'; if(*arg && inquote==0) notyetfinished=0; } break; case '#': notyetfinished=0; break; case '"': if(inword) error_at_line(EXIT_FAILURE, 0, filename, lineno, "Quotes have to be surrounded by whitespace " "characters (space, tab, new line, etc)."); if(inquote) { *line='\0'; inquote=0; notyetfinished=0; } else { if(*name==NULL) error_at_line(EXIT_FAILURE, 0, filename, lineno, "option name should not start with " "double quotes (\")."); inquote=1; *arg=line+1; } break; default: if(inword==0 && inquote==0) { if(*name==NULL) *name=line; else /* *name is set, now assign *arg. */ *arg=line; inword=1; } break; } while(*(++line)!='\0' && notyetfinished); /* In the last line of the file, there is no new line to be converted to a '\0' character! So if value has been assigned, we are not in a quote and the line has finished, it means the given value has also finished. */ if(*line=='\0' && *arg && inquote==0) notyetfinished=0; /* This was a blank line: */ if(*name==NULL && *arg==NULL) return; /* Name or value were set but not yet finished. */ if(notyetfinished) error_at_line(EXIT_FAILURE, 0, filename, lineno, "line finished before option name and value could " "be read."); } static int options_set_from_name(char *name, char *arg, struct argp_option *options, struct gal_options_common_params *cp, char *filename, size_t lineno) { size_t i; /* Go through all the options and find the one that should keep this value, then put its value into the appropriate key. Note that the options array finishs with an all zero element, so we don't need to know the number before hand.*/ for(i=0;1;++i) { /* Check if the key corresponds to this option. */ if( options[i].name && !strcmp(options[i].name, name) ) { /* Ignore this option and its value. This can happen in several situations: - Not all common options are used by all programs. When a program doesn't use an option, it will be given an `OPTION_HIDDEN' flag. There is no point in reading the values of such options. - When the option already has a value AND it ISN'T a linked list. */ if( options[i].flags==OPTION_HIDDEN || ( options[i].set && !gal_type_is_list(options[i].type ) ) ) return 0; /* Read the value into the option and do a sanity check. */ gal_options_read_check(&options[i], arg, filename, lineno, cp); /* We have found and set the value given to this option, so just return success (an error_t of 0 means success). */ return 0; } else { /* The last option has all its values set to zero. If we get to this point then the given name was not recognized and this function will return a 1. */ if(gal_options_is_last(&options[i])) return 1; } } } /* If the last config option has a value which is 1, then in some previous configuration file the user has asked to stop parsing configuration files. In that case, don't read this configuration file. */ static int options_lastconfig_has_been_called(struct argp_option *coptions) { size_t i; for(i=0; !gal_options_is_last(&coptions[i]); ++i) if( coptions[i].key == GAL_OPTIONS_KEY_LASTCONFIG && coptions[i].set && *((unsigned char *)(coptions[i].value)) ) return 1; return 0; } static void options_parse_file(char *filename, struct gal_options_common_params *cp, int enoent_abort) { FILE *fp; char *line, *name, *arg; size_t linelen=10, lineno=0; /* If `lastconfig' was called prior to this file, then just return and ignore this configuration file. */ if( options_lastconfig_has_been_called(cp->coptions) ) return; /* Open the file. If the file doesn't exist, then just ignore the configuration file and return. */ errno=0; fp=fopen(filename, "r"); if(fp==NULL) { if(errno==ENOENT && enoent_abort==0) return; else error(EXIT_FAILURE, errno, "%s: to be read as a configuration file", filename); } /* Allocate the space necessary to keep a copy of each line as we parse it. Note that `getline' is going to later `realloc' this space to fit the line length. */ errno=0; line=malloc(linelen*sizeof *line); if(line==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `line'", __func__, linelen*sizeof *line); /* Read the parameters line by line. */ while( getline(&line, &linelen, fp) != -1 ) { ++lineno; if( gal_txt_line_stat(line) == GAL_TXT_LINESTAT_DATAROW ) { /* Get the option name and argument/value. */ options_read_name_arg(line, filename, lineno, &name, &arg); /* First look into this program's options, if the option isn't found there, `options_set_from_name' will return 1. So the condition will succeed and we will start looking into the common options, if it isn't found there either, then report an error.*/ if( options_set_from_name(name, arg, cp->poptions, cp, filename, lineno) ) if( options_set_from_name(name, arg, cp->coptions, cp, filename, lineno) ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "unrecognized option `%s', for the full list of " "options, please run with `--help'", name); } } /* Close the file. */ errno=0; if(fclose(fp)) error(EXIT_FAILURE, errno, "%s: couldn't close after reading as " "a configuration file in %s", filename, __func__); /* Clean up and return. */ free(line); } /* This function will be used when the `--config' option is called. */ void * gal_options_call_parse_config_file(struct argp_option *option, char *arg, char *filename, size_t lineno, void *cp) { /* Call the confguration file parser. */ options_parse_file(arg, cp, 1); /* Just to avoid compiler warnings, then return, note that all pointers are just copies. */ option=NULL; filename=NULL; lineno=0; return NULL; } /* Read the configuration files and put the values of the options not given into it. The directories containing the configuration files are fixed for all the programs. - `SYSCONFIG_DIR' is passed onto the library functions at compile time from the command-line. You can search for it in the outputs of `make'. The main reason is that we want the the user still has the chance to change the installation directory after `configure'. - `USERCONFIG_DIR' is defined in `config.h'. - `CURDIRCONFIG_DIR' is defined in `config.h'. */ static void gal_options_parse_config_files(struct gal_options_common_params *cp) { char *home; char *filename; /* A small sanity check because in multiple places, we have assumed the on/off options have a type of `unsigned char'. */ if(GAL_OPTIONS_NO_ARG_TYPE != GAL_TYPE_UINT8) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can fix " "the problem. `GAL_OPTIONS_NO_ARG_TYPE' must be the " "`uint8' type", __func__, PACKAGE_BUGREPORT); /* The program's current directory configuration file. */ asprintf(&filename, ".%s/%s.conf", PACKAGE, cp->program_exec); options_parse_file(filename, cp, 0); free(filename); /* Common options configuration file. */ asprintf(&filename, ".%s/%s.conf", PACKAGE, PACKAGE); options_parse_file(filename, cp, 0); free(filename); /* Read the home environment variable. */ home=options_get_home(); /* The program's user-wide configuration file. */ asprintf(&filename, "%s/%s/%s.conf", home, USERCONFIG_DIR, cp->program_exec); options_parse_file(filename, cp, 0); free(filename); /* Common options user-wide configuration file. */ asprintf(&filename, "%s/%s/%s.conf", home, USERCONFIG_DIR, PACKAGE); options_parse_file(filename, cp, 0); free(filename); /* The program's system-wide configuration file. */ asprintf(&filename, "%s/%s.conf", SYSCONFIG_DIR, cp->program_exec); options_parse_file(filename, cp, 0); free(filename); /* Common options system-wide configuration file. */ asprintf(&filename, "%s/%s.conf", SYSCONFIG_DIR, PACKAGE); options_parse_file(filename, cp, 0); free(filename); } static void options_reverse_lists_check_mandatory(struct gal_options_common_params *cp, struct argp_option *options) { size_t i; for(i=0; !gal_options_is_last(&options[i]); ++i) { if(options[i].set) switch(options[i].type) { case GAL_TYPE_STRLL: gal_list_str_reverse( (gal_list_str_t **)(options[i].value) ); break; } else if(options[i].mandatory==GAL_OPTIONS_MANDATORY) gal_options_add_to_not_given(cp, &options[i]); } } /* Read all configuration files and set common options */ void gal_options_read_config_set(struct gal_options_common_params *cp) { /* Parse all the configuration files. */ gal_options_parse_config_files(cp); /* Reverse the order of all linked list type options so the popping order is the same as the user's input order. We need to do this here because when printing those options, their order matters.*/ options_reverse_lists_check_mandatory(cp, cp->poptions); options_reverse_lists_check_mandatory(cp, cp->coptions); /* Abort if any of the mandatory options are not set. */ gal_options_abort_if_mandatory_missing(cp); /* If `numthreads' is 0, use the number of threads available to the system. */ if(cp->numthreads==0) cp->numthreads=gal_threads_number(); } /**********************************************************************/ /************ Printing/Writing ***************/ /**********************************************************************/ /* We don't want to print the values of configuration specific options and the output option. The output value is assumed to be specific to each input, and the configuration options are for reading the configuration, not writing it. */ static int option_is_printable(struct argp_option *option) { /* Use non-key fields: - If option is hidden (not relevant to this program). - Options with an INVALID type are not to be printed (they are probably processed to a higher level value with functions). */ if( (option->flags & OPTION_HIDDEN) || option->type==GAL_TYPE_INVALID ) return 0; /* Then check if it is a pre-program option. */ switch(option->key) { case GAL_OPTIONS_KEY_OUTPUT: case GAL_OPTIONS_KEY_CITE: case GAL_OPTIONS_KEY_PRINTPARAMS: case GAL_OPTIONS_KEY_CONFIG: case GAL_OPTIONS_KEY_SETDIRCONF: case GAL_OPTIONS_KEY_SETUSRCONF: case GAL_OPTIONS_KEY_LASTCONFIG: return 0; } return 1; } /* For a given type, print the value in `ptr' in a space of `width' elements. If `width==0', then return the width necessary to print the value. */ static int options_print_any_type(struct argp_option *option, void *ptr, int type, int width, FILE *fp, struct gal_options_common_params *cp) { char *str; /* Write the value into a string. */ str = ( option->func ? option->func(option, NULL, NULL, (size_t)(-1), cp->program_struct) : gal_type_to_string(ptr, type, 1) ); /* If only the width was desired, don't actually print the string, just return its length. Otherwise, print it. */ if(width) fprintf(fp, "%-*s ", width, str); else width=strlen(str); /* Free the allocated space and return. */ free(str); return width; } /* An option structure is given, return its name and value print lengths. */ static void options_correct_max_lengths(struct argp_option *option, int *max_nlen, int *max_vlen, struct gal_options_common_params *cp) { int vlen; gal_list_str_t *tmp; /* Invalid types are set for functions that don't save the raw user input, but do higher-level analysis on them for storing. */ if(option->type==GAL_TYPE_INVALID) return; /* Get the length of the value and save its length length if its larger than the widest value. */ if(gal_type_is_list(option->type)) { /* A small sanity check. */ if(option->type!=GAL_TYPE_STRLL) error(EXIT_FAILURE, 0, "%s: currently only string linked lists " "are acceptable for printing", __func__); /* Check each node, one by one. */ for(tmp=*(gal_list_str_t **)(option->value); tmp!=NULL; tmp=tmp->next) { /* Get the length of this node: */ vlen=options_print_any_type(option, &tmp->v, GAL_TYPE_STRING, 0, NULL, cp); /* If its larger than the maximum length, then put it in. */ if( vlen > *max_vlen ) *max_vlen=vlen; } } else { vlen=options_print_any_type(option, option->value, option->type, 0, NULL, cp); if( vlen > *max_vlen ) *max_vlen=vlen; } /* If the name of this option is larger than all existing, set its length as the largest name length. */ if( strlen(option->name) > *max_nlen ) *max_nlen = strlen(option->name); } /* To print the options nicely, we need the maximum lengths of the options and their values. */ static void options_set_lengths(struct argp_option *poptions, struct argp_option *coptions, int *namelen, int *valuelen, struct gal_options_common_params *cp) { int i, max_nlen=0, max_vlen=0; /* For program specific options. */ for(i=0; !gal_options_is_last(&poptions[i]); ++i) if(poptions[i].name && poptions[i].set) options_correct_max_lengths(&poptions[i], &max_nlen, &max_vlen, cp); /* For common options. Note that the options that will not be printed are in this category, so we also need to check them. The detailed steps are the same as before. */ for(i=0; !gal_options_is_last(&coptions[i]); ++i) if( coptions[i].name && coptions[i].set && option_is_printable(&coptions[i]) ) options_correct_max_lengths(&coptions[i], &max_nlen, &max_vlen, cp); /* Save the final values in the output pointers. */ *namelen = max_nlen; *valuelen = ( max_vlen < GAL_OPTIONS_MAX_VALUE_LEN ? max_vlen : GAL_OPTIONS_MAX_VALUE_LEN ); } /* The `#' before the `doc' string are not required by the configuration file parser when the documentation string fits in a line. However, when the `doc' string is longer than 80 characters, it will be cut between multiple lines and without the `#', the start of the line will be read as an option. */ static void options_print_doc(FILE *fp, const char *doc, int nvwidth) { size_t len=strlen(doc); /* The `+3' is because of the three extra spaces in this line: one before the variable name, one after it and one after the value. */ int i, prewidth=nvwidth+3, width=77-prewidth, cwidth; /* We only want the formatting when writing to stdout. */ if(lennext) { fprintf(fp, " %-*s ", namewidth, options[i].name); options_print_any_type(&options[i], &tmp->v, GAL_TYPE_STRING, valuewidth, fp, cp); options_print_doc(fp, options[i].doc, namewidth+valuewidth); } /* Normal types. */ else { fprintf(fp, " %-*s ", namewidth, options[i].name); options_print_any_type(&options[i], options[i].value, options[i].type, valuewidth, fp, cp); options_print_doc(fp, options[i].doc, namewidth+valuewidth); } } } static void options_print_all(struct gal_options_common_params *cp, char *dirname, const char *optionname) { size_t i; FILE *fp; time_t rawtime; char *topicstr, *filename; gal_list_i32_t *group=NULL; gal_list_str_t *topic=NULL; int groupint, namelen, valuelen; struct argp_option *coptions=cp->coptions, *poptions=cp->poptions; /* If the configurations are to be written to a file, then do the preparations. */ if(dirname) { /* Make the host directory if it doesn't already exist. */ gal_checkset_mkdir(dirname); /* Prepare the full filename: */ asprintf(&filename, "%s/%s.conf", dirname, cp->program_exec); /* Remove the file if it already exists. */ gal_checkset_writable_remove(filename, 0, 0); /* Open the file for writing */ errno=0; fp=fopen(filename, "w"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s: couldn't open to write " "configuration file in %s", dirname, __func__); /* Print the basic information as comments in the file first. */ time(&rawtime); fprintf(fp, "# %s (%s) %s.\n" "# Written at %s#\n" "# - Empty lines are ignored.\n" "# - Lines starting with `#` are ignored.\n" "# - The long option name is followed by a value.\n" "# - The name and value should be separated by atleast\n" "# one white space character (for example space or tab).\n" "# - If the value has space, enclose the whole value in\n" "# double quotation (\") signs.\n" "# - After the value, the rest of the line is ignored.\n" "#\n# Run `info %s' for a more elaborate description of each " "option.\n", cp->program_name, PACKAGE_NAME, PACKAGE_VERSION, ctime(&rawtime), cp->program_exec); } else fp=stdout; /* Parse all the options with a title, note that the `Input', `Output' and `Operating mode' options are defined in the common options, while the (possible) other groups are in the program specific options. We will only be dealing with the `topics' linked list in this function and the strings in `poption' are statically allocated, so its fine to not waste CPU cycles allocating and freeing.*/ for(i=0; !gal_options_is_last(&coptions[i]); ++i) if(coptions[i].name==NULL && coptions[i].key==0 && coptions[i].doc) { /* The `(char *)' is because `.doc' is a constant and this helps remove the compiler warning. */ gal_list_i32_add(&group, coptions[i].group); gal_list_str_add(&topic, (char *)coptions[i].doc, 0); } for(i=0; !gal_options_is_last(&poptions[i]); ++i) if(poptions[i].name==NULL && poptions[i].key==0 && poptions[i].doc) { gal_list_i32_add(&group, poptions[i].group); gal_list_str_add(&topic, (char *)poptions[i].doc, 0); } /* Reverse the linked lists to get the same input order. */ gal_list_str_reverse(&topic); gal_list_i32_reverse(&group); /* Get the maximum width of names and values. */ options_set_lengths(poptions, coptions, &namelen, &valuelen, cp); /* Go over each topic and print every option that is in this group. */ while(topic) { /* Pop the nodes from the linked list. */ groupint = gal_list_i32_pop(&group); topicstr = gal_list_str_pop(&topic); /* First print the topic, */ fprintf(fp, "\n# %s\n", topicstr); /* fprintf(fp, "# "); i=0; while(i++program_name, optionname); free(filename); } /* Exit the program successfully */ exit(EXIT_SUCCESS); } #define OPTIONS_UINT8VAL *(uint8_t *)(cp->coptions[i].value) void gal_options_print_state(struct gal_options_common_params *cp) { size_t i; unsigned char sum=0; char *home, *dirname; /* A sanity check is necessary first. We want to make sure that the user hasn't called more than one of these options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) if(cp->coptions[i].set) switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_PRINTPARAMS: case GAL_OPTIONS_KEY_SETDIRCONF: case GAL_OPTIONS_KEY_SETUSRCONF: sum += OPTIONS_UINT8VAL; } if(sum>1) error(EXIT_FAILURE, 0, "only one of the `printparams', `setdirconf' " "and `setusrconf' options can be called in each run"); /* Print the required configuration files. Note that simply having a non-NULL value is not enough. They can have a value of 1 or 0, and the respective file should only be created if we have a value of 1. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) if(cp->coptions[i].set && OPTIONS_UINT8VAL) switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_PRINTPARAMS: options_print_all(cp, NULL, NULL); break; case GAL_OPTIONS_KEY_SETDIRCONF: asprintf(&dirname, ".%s", PACKAGE); options_print_all(cp, dirname, cp->coptions[i].name); free(dirname); break; case GAL_OPTIONS_KEY_SETUSRCONF: home=options_get_home(); asprintf(&dirname, "%s/%s", home, USERCONFIG_DIR); options_print_all(cp, dirname, cp->coptions[i].name); free(dirname); break; } } gnuastro-0.5/lib/match.c0000644000175000017500000006313213216276304012160 00000000000000/********************************************************************* match -- Functions to match catalogs and WCS. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include /**********************************************************************/ /***************** Coordinate match custom list *******************/ /**********************************************************************/ struct match_coordinate_sfll { float f; size_t v; struct match_coordinate_sfll *next; }; static void match_coordinate_add_to_sfll(struct match_coordinate_sfll **list, size_t value, float fvalue) { struct match_coordinate_sfll *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: new node couldn't be allocated", __func__); newnode->v=value; newnode->f=fvalue; newnode->next=*list; *list=newnode; } static void match_coordinate_pop_from_sfll(struct match_coordinate_sfll **list, size_t *value, float *fvalue) { struct match_coordinate_sfll *tmp; tmp=*list; *value=tmp->v; *fvalue=tmp->f; *list=tmp->next; free(tmp); } /********************************************************************/ /************* Coordinate matching *************/ /************* Sanity checks and preparations *************/ /********************************************************************/ /* Since these checks are repetative, its easier to have a separate function for both inputs. */ static void match_coordinate_sanity_check_columns(gal_data_t *coord, char *info, int inplace, int *allf64) { gal_data_t *tmp; for(tmp=coord; tmp!=NULL; tmp=tmp->next) { if(tmp->type!=GAL_TYPE_FLOAT64) { if(inplace) error(EXIT_FAILURE, 0, "%s: when `inplace' is activated, the " "input coordinates must have `float64' type. At least " "one node of the %s list has type of `%s'", __func__, info, gal_type_name(tmp->type, 1)); else *allf64=0; } if(tmp->ndim!=1) error(EXIT_FAILURE, 0, "%s: each input coordinate column must have " "a single dimension (be a single column). Atleast one node of " "the %s list has %zu dimensions", __func__, info, tmp->ndim); if(tmp->size!=coord->size) error(EXIT_FAILURE, 0, "%s: the nodes of each list of coordinates " "must have the same number of elements. At least one node of " "the %s list has %zu elements while the first has %zu " "elements", __func__, info, tmp->size, coord->size); } } /* To keep the main function clean, we'll do the sanity checks here. */ static void match_coordinaes_sanity_check(gal_data_t *coord1, gal_data_t *coord2, double *aperture, int inplace, int *allf64) { size_t ncoord1=gal_list_data_number(coord1); /* Make sure both lists have the same number of datasets. NOTE: they don't need to have the same number of elements. */ if( ncoord1!=gal_list_data_number(coord2) ) error(EXIT_FAILURE, 0, "%s: the two inputs have different numbers of " "datasets (%zu and %zu respectively)", __func__, ncoord1, gal_list_data_number(coord2)); /* This function currently only works on 1 and 2 dimensional inputs. */ if(ncoord1>2) error(EXIT_FAILURE, 0, "%s: %zu dimension matching requested, this " "function currently only matches datasets with a maximum of 2 " "dimensions", __func__, ncoord1); /* Check the column properties. */ match_coordinate_sanity_check_columns(coord1, "first", inplace, allf64); match_coordinate_sanity_check_columns(coord2, "second", inplace, allf64); /* Check the aperture values. */ if(aperture[0]<=0) error(EXIT_FAILURE, 0, "%s: the first value in the aperture (%g) cannot " "be zero or negative", __func__, aperture[0]); if(ncoord1==2) if(aperture[1]<=0 || aperture[1]>1) error(EXIT_FAILURE, 0, "%s: the second value in the aperture (%g) " "is the axis ratio, so it must be larger than zero and less " "than 1", __func__, aperture[1]); } /* To keep things clean, the sorting of each input array will be done in this function. */ static size_t * match_coordinates_prepare_sort(gal_data_t *coords, size_t minmapsize) { gal_data_t *tmp; size_t *permutation=gal_data_malloc_array(GAL_TYPE_SIZE_T, coords->size, __func__, "permutation"); /* Get the permutation necessary to sort all the columns (based on the first column). */ gsl_sort_index(permutation, coords->array, 1, coords->size); /* Sort all the coordinates. */ for(tmp=coords; tmp!=NULL; tmp=tmp->next) gal_permutation_apply(tmp, permutation); /* Clean up. */ return permutation; } /* Do the preparations for matching of coordinates. */ static void match_coordinates_prepare(gal_data_t *coord1, gal_data_t *coord2, int sorted_by_first, int inplace, int allf64, gal_data_t **A_out, gal_data_t **B_out, size_t **A_perm, size_t **B_perm, size_t minmapsize) { gal_data_t *c, *tmp, *A=NULL, *B=NULL; /* Sort the datasets if they aren't sorted. If the dataset is already sorted, then `inplace' is irrelevant. */ if(sorted_by_first && allf64) { *A_out=coord1; *B_out=coord2; } else { /* Allocating a new list is only necessary when `inplace==0' or all the columns are double. */ if( inplace && allf64 ) { *A_out=coord1; *B_out=coord2; } else { /* Copy the first list. */ for(tmp=coord1; tmp!=NULL; tmp=tmp->next) { c=gal_data_copy(tmp); c->next=NULL; gal_list_data_add(&A, c); } /* Copy the second list. */ for(tmp=coord2; tmp!=NULL; tmp=tmp->next) { c=gal_data_copy(tmp); c->next=NULL; gal_list_data_add(&B, c); } /* Reverse both lists: the copying process reversed the order. */ gal_list_data_reverse(&A); gal_list_data_reverse(&B); /* Set the output pointers. */ *A_out=A; *B_out=B; } /* Sort each dataset by the first coordinate. */ *A_perm = match_coordinates_prepare_sort(*A_out, minmapsize); *B_perm = match_coordinates_prepare_sort(*B_out, minmapsize); } } /********************************************************************/ /************* Coordinate matching *************/ /********************************************************************/ static double match_coordinates_elliptical_r_2d(double d1, double d2, double *ellipse, double c, double s) { double Xr = d1 * ( c ) + d2 * ( s ); double Yr = d1 * ( -1.0f*s ) + d2 * ( c ); return sqrt( Xr*Xr + Yr*Yr/ellipse[1]/ellipse[1] ); } static double match_coordinates_distance(double *delta, int iscircle, size_t ndim, double *aperture, double c, double s) { /* For more than one dimension, we'll need to calculate the distance from the deltas (differences) in each dimension. */ switch(ndim) { case 1: return fabs(delta[0]); case 2: return ( iscircle ? sqrt( delta[0]*delta[0] + delta[1]*delta[1] ) : match_coordinates_elliptical_r_2d(delta[0], delta[1], aperture, c, s) ); default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to fix " "the problem. The value %zu is not recognized for ndim", __func__, PACKAGE_BUGREPORT, ndim); } /* Control should not reach this point. */ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to fix the " "problem. Control should not reach the end of this function", __func__, PACKAGE_BUGREPORT); return NAN; } /* Go through both catalogs and find which records/rows in the second catalog (catalog b) are within the acceptable distance of each record in the first (a). */ static void match_coordinates_second_in_first(gal_data_t *A, gal_data_t *B, double *aperture, struct match_coordinate_sfll **bina) { /* To keep things easy to read, all variables related to catalog 1 start with an `a' and things related to catalog 2 are marked with a `b'. The redundant variables (those that equal a previous value) are only defined to make it easy to read the code.*/ int iscircle=0; double r, c=NAN, s=NAN; size_t i, ar=A->size, br=B->size; size_t ai, bi, blow=0, prevblow=0; size_t ndim=gal_list_data_number(A); double dist[2]={NAN,NAN}, delta[2]={NAN,NAN}; double *a[2]={A->array, A->next ? A->next->array : NULL}; double *b[2]={B->array, B->next ? B->next->array : NULL}; /* See if the aperture is a circle or not. */ switch(ndim) { case 1: iscircle = 0; /* Irrelevant for 1D. */ break; case 2: iscircle = aperture[1]==1 ? 1 : 0; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to fix " "the problem. The value %zu is not recognized for ndim", __func__, PACKAGE_BUGREPORT, ndim); } /* Preparations for the shape of the aperture. */ if(ndim==1 || iscircle) dist[0]=dist[1]=aperture[0]; else { /* Using the box that encloses the aperture, calculate the distance along each axis. */ gal_box_bound_ellipse_extent(aperture[0], aperture[0]*aperture[1], aperture[2], dist); /* Calculate the sin and cos of the given ellipse if necessary for ease of processing later. */ c = cos( aperture[2] * M_PI/180.0 ); s = sin( aperture[2] * M_PI/180.0 ); } /* For each row/record of catalog `a', make a list of the nearest records in catalog b within the maximum distance. Note that both catalogs are sorted by their first axis coordinate.*/ for(ai=0;ai= a[1][ai]-dist[1] && b[1][bi] <= a[1][ai]+dist[1] ) ) { /* Now, `bi' is within the rectangular range of `ai'. But this is not enough to consider the two objects matched for the following reasons: 1) Until now we have avoided calculations other than larger or smaller on double precision floating point variables for efficiency. So the `bi' is within a square of side `dist[0]*dist[1]' around `ai' (not within a fixed radius). 2) Other objects in the `b' catalog may be closer to `ai' than this `bi'. 3) The closest `bi' to `ai' might be closer to another catalog `a' record. To address these problems, we will use a linked list to keep the indexes of the `b's near `ai', along with their distance. We only add the `bi's to this list that are within the acceptable distance. Since we are dealing with much fewer objects at this stage, it is justified to do complex mathematical operations like square root and multiplication. This fixes the first problem. The next two problems will be solved with the list after parsing of the whole catalog is complete.*/ for(i=0;inext) printf("%lu: %f\n", tmp->v, tmp->f); } */ } } /* In `match_coordinates_second_in_first', we made an array of lists, here we want to reverse that list to fix the second two issues that were discussed there. */ void match_coordinates_rearrange(gal_data_t *A, gal_data_t *B, struct match_coordinate_sfll **bina) { size_t bi; float *fp, *fpf, r, *ainb; size_t ai, ar=A->size, br=B->size; /* Allocate the space for `ainb' and initialize it to NaN (since zero is meaningful) in this context (both for indexs and also for floats). This is a two column array that will keep the distance and index of the closest element in catalog `a' for each element in catalog b. */ errno=0; ainb=calloc(2*br, sizeof *ainb); if(ainb==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for `ainb'", __func__, br*sizeof *ainb); fpf=(fp=ainb)+2*br; do *fp++=NAN; while(fpf ) { bina[ai]->f=r; bina[ai]->v=bi; } } else match_coordinate_add_to_sfll(&bina[ai], bi, r); } /* For checking the status of affairs uncomment this block { size_t bi, counter=0; double *a[2]={A->array, A->next->array}; double *b[2]={B->array, B->next->array}; printf("Rearranged bina:\n"); for(ai=0;aiv; printf("A_%lu (%.8f, %.8f) <--> B_%lu (%.8f, %.8f):\n\t%f\n", ai, a[0][ai], a[1][ai], bi, b[0][bi], b[1][bi], bina[ai]->f); } printf("\n-----------\nMatched: %zu\n", counter); } exit(0); */ /* Clean up */ free(ainb); } /* The matching has been done, write the output. */ static gal_data_t * gal_match_coordinates_output(gal_data_t *A, gal_data_t *B, size_t *A_perm, size_t *B_perm, struct match_coordinate_sfll **bina, size_t minmapsize) { float r; double *rval; gal_data_t *out; uint8_t *Bmatched; size_t ai, bi, nummatched=0; size_t *aind, *bind, match_i, nomatch_i; /* Find how many matches there were in total */ for(ai=0;aisize;++ai) if(bina[ai]) ++nummatched; /* If there aren't any matches, return NULL. */ if(nummatched==0) return NULL; /* Allocate the output list. */ out=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 1, &A->size, NULL, 0, minmapsize, "CAT1_ROW", "counter", "Row index in first catalog (counting from 0)."); out->next=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 1, &B->size, NULL, 0, minmapsize, "CAT2_ROW", "counter", "Row index in second catalog (counting " "from 0)."); out->next->next=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &nummatched, NULL, 0, minmapsize, "MATCH_DIST", NULL, "Distance between the match."); /* Allocate the `Bmatched' array which is a flag for which rows of the second catalog were matched. The columns that had a match will get a value of one while we are parsing them below. */ Bmatched=gal_data_calloc_array(GAL_TYPE_UINT8, B->size, __func__, "Bmatched"); /* Initialize the indexs. We want the first `nummatched' indexs in both outputs to be the matching rows. The non-matched rows should start to be indexed after the matched ones. So the first non-matched index is at the index `nummatched'. */ match_i = 0; nomatch_i = nummatched; /* Fill in the output arrays. */ aind = out->array; bind = out->next->array; rval = out->next->next->array; for(ai=0;aisize;++ai) { /* A match was found. */ if(bina[ai]) { /* Note that the permutation keeps the original indexs. */ match_coordinate_pop_from_sfll(&bina[ai], &bi, &r); rval[ match_i ] = r; aind[ match_i ] = A_perm ? A_perm[ai] : ai; bind[ match_i++ ] = B_perm ? B_perm[bi] : bi; /* Set a `1' for this object in the second catalog. This will later be used to find which rows didn't match to fill in the output.. */ Bmatched[ B_perm ? B_perm[bi] : bi ] = 1; } /* No match found. At this stage, we can only fill the indexs of the first input. The second input needs to be matched afterwards.*/ else aind[ nomatch_i++ ] = A_perm ? A_perm[ai] : ai; } /* Complete the second input's permutation. */ nomatch_i=nummatched; for(bi=0;bisize;++bi) if( Bmatched[bi] == 0 ) bind[ nomatch_i++ ] = bi; /* For a check printf("\nFirst input's permutation:\n"); for(ai=0;aisize;++ai) printf("%s%zu\n", aisize;++bi) printf("%s%zu\n", bisize' elements (pointers) and for each, it keeps a list of `b' elements that are nearest to it. */ errno=0; bina=calloc(A->size, sizeof *bina); if(bina==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for `bina'", __func__, A->size*sizeof *bina); /* All records in `b' that match each `a' (possibly duplicate). */ match_coordinates_second_in_first(A, B, aperture, bina); /* Two re-arrangings will fix the issue. */ match_coordinates_rearrange(A, B, bina); /* The match is done, write the output. */ out=gal_match_coordinates_output(A, B, A_perm, B_perm, bina, minmapsize); /* Clean up. */ free(bina); if(A!=coord1) { gal_list_data_free(A); gal_list_data_free(B); } if(A_perm) free(A_perm); if(B_perm) free(B_perm); /* Set `nummatched' and return output. */ *nummatched = out ? out->next->next->size : 0; return out; } gnuastro-0.5/lib/list.c0000644000175000017500000005206413121462410012027 00000000000000/********************************************************************* Functions for linked lists. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include /**************************************************************** ***************** String ******************** ****************************************************************/ void gal_list_str_add(gal_list_str_t **list, char *value, int allocate) { gal_list_str_t *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); if(allocate) gal_checkset_allocate_copy(value, &newnode->v); else newnode->v=value; newnode->next=*list; *list=newnode; } char * gal_list_str_pop(gal_list_str_t **list) { char *out=NULL; gal_list_str_t *tmp; if(*list) { tmp=*list; out=tmp->v; *list=tmp->next; free(tmp); } return out; } size_t gal_list_str_number(gal_list_str_t *list) { size_t num=0; gal_list_str_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_list_str_print(gal_list_str_t *list) { gal_list_str_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("%s\n", tmp->v); } void gal_list_str_reverse(gal_list_str_t **list) { char *thisstring; gal_list_str_t *correctorder=NULL; /* Only do the reversal if there is more than one element. */ if( *list && (*list)->next ) { while(*list!=NULL) { thisstring=gal_list_str_pop(list); gal_list_str_add(&correctorder, thisstring, 0); } *list=correctorder; } } void gal_list_str_free(gal_list_str_t *list, int freevalue) { gal_list_str_t *tmp; while(list!=NULL) { tmp=list->next; if(freevalue) free(list->v); free(list); list=tmp; } } /**************************************************************** ***************** int ******************** ****************************************************************/ void gal_list_i32_add(gal_list_i32_t **list, int32_t value) { gal_list_i32_t *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->next=*list; *list=newnode; } int32_t gal_list_i32_pop(gal_list_i32_t **list) { gal_list_i32_t *tmp; int out=GAL_BLANK_INT32; if(*list) { tmp=*list; out=tmp->v; *list=tmp->next; free(tmp); } return out; } size_t gal_list_i32_number(gal_list_i32_t *list) { size_t num=0; gal_list_i32_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_list_i32_print(gal_list_i32_t *list) { gal_list_i32_t *tmp; for(tmp=list; tmp!=NULL; tmp=tmp->next) printf("%"PRId32"\n", tmp->v); } void gal_list_i32_reverse(gal_list_i32_t **list) { int thisnum; gal_list_i32_t *correctorder=NULL; if( *list && (*list)->next ) { while(*list!=NULL) { thisnum=gal_list_i32_pop(list); gal_list_i32_add(&correctorder, thisnum); } *list=correctorder; } } int32_t * gal_list_i32_to_array(gal_list_i32_t *list, int reverse, size_t *num) { size_t i; int32_t *out=NULL; gal_list_i32_t *tmp; *num=gal_list_i32_number(list); if(*num) { out=gal_data_malloc_array(GAL_TYPE_SIZE_T, *num, __func__, "out"); i = reverse ? *num-1: 0; if(reverse) for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i--]=tmp->v; else for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i++]=tmp->v; } return out; } void gal_list_i32_free(gal_list_i32_t *list) { gal_list_i32_t *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** ***************** size_t ******************** ****************************************************************/ void gal_list_sizet_add(gal_list_sizet_t **list, size_t value) { gal_list_sizet_t *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->next=*list; *list=newnode; } size_t gal_list_sizet_pop(gal_list_sizet_t **list) { gal_list_sizet_t *tmp; size_t out=GAL_BLANK_SIZE_T; if(list) { tmp=*list; out=tmp->v; *list=tmp->next; free(tmp); } return out; } size_t gal_list_sizet_number(gal_list_sizet_t *list) { size_t num=0; gal_list_sizet_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_list_sizet_print(gal_list_sizet_t *list) { gal_list_sizet_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) printf("%zu\n", tmp->v); return; } void gal_list_sizet_reverse(gal_list_sizet_t **list) { size_t thisnum; gal_list_sizet_t *correctorder=NULL; if( *list && (*list)->next ) { while(*list!=NULL) { thisnum=gal_list_sizet_pop(list); gal_list_sizet_add(&correctorder, thisnum); } *list=correctorder; } } size_t * gal_list_sizet_to_array(gal_list_sizet_t *list, int reverse, size_t *num) { size_t i, *out=NULL; gal_list_sizet_t *tmp; *num=gal_list_sizet_number(list); if(*num) { out=gal_data_malloc_array(GAL_TYPE_SIZE_T, *num, __func__, "out"); i = reverse ? *num-1: 0; if(reverse) for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i--]=tmp->v; else for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i++]=tmp->v; } return out; } void gal_list_sizet_free(gal_list_sizet_t *list) { gal_list_sizet_t *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** ***************** Float ******************** ****************************************************************/ void gal_list_f32_add(gal_list_f32_t **list, float value) { struct gal_list_f32_t *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->next=*list; *list=newnode; } float gal_list_f32_pop(gal_list_f32_t **list) { float out=NAN; gal_list_f32_t *tmp; if(*list) { tmp=*list; out=tmp->v; *list=tmp->next; free(tmp); } return out; } size_t gal_list_f32_number(gal_list_f32_t *list) { size_t num=0; gal_list_f32_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_list_f32_reverse(gal_list_f32_t **list) { float thisnum; gal_list_f32_t *correctorder=NULL; if( *list && (*list)->next ) { while(*list!=NULL) { thisnum=gal_list_f32_pop(list); gal_list_f32_add(&correctorder, thisnum); } *list=correctorder; } } void gal_list_f32_print(gal_list_f32_t *list) { gal_list_f32_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) printf("%f\n", tmp->v); return; } float * gal_list_f32_to_array(gal_list_f32_t *list, int reverse, size_t *num) { size_t i; float *out=NULL; gal_list_f32_t *tmp; /* Find the number of elements: */ *num=gal_list_f32_number(list); /* If there is actually anything in the list, then allocate the array and fill it in. */ if(*num) { /* Allocate the space: */ out=gal_data_malloc_array(GAL_TYPE_FLOAT32, *num, __func__, "out"); /* Fill in the array. */ i = reverse ? *num-1: 0; if(reverse) for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i--]=tmp->v; else for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i++]=tmp->v; } /* Return the created array. */ return out; } void gal_list_f32_free(gal_list_f32_t *list) { gal_list_f32_t *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** ***************** Double ******************** ****************************************************************/ void gal_list_f64_add(gal_list_f64_t **list, double value) { gal_list_f64_t *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->next=*list; *list=newnode; } double gal_list_f64_pop(gal_list_f64_t **list) { double out=NAN; gal_list_f64_t *tmp; if(*list) { tmp=*list; out=tmp->v; *list=tmp->next; free(tmp); } return out; } size_t gal_list_f64_number(gal_list_f64_t *list) { size_t num=0; gal_list_f64_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_list_f64_print(gal_list_f64_t *list) { gal_list_f64_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) printf("%f\n", tmp->v); return; } void gal_list_f64_reverse(gal_list_f64_t **list) { double thisvalue; gal_list_f64_t *correctorder=NULL; /* Only do the reversal if there is more than one element. */ if( *list && (*list)->next ) { while(*list!=NULL) { thisvalue=gal_list_f64_pop(list); gal_list_f64_add(&correctorder, thisvalue); } *list=correctorder; } } double * gal_list_f64_to_array(gal_list_f64_t *list, int reverse, size_t *num) { size_t i; double *out=NULL; gal_list_f64_t *tmp; /* Find the number of elements: */ *num=gal_list_f64_number(list); /* If there is actually anything in the list, then allocate the array and fill it in. */ if(*num) { /* Allocate the space: */ out=gal_data_malloc_array(GAL_TYPE_FLOAT64, *num, __func__, "out"); /* Fill in the array. */ i = reverse ? *num-1: 0; if(reverse) for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i--]=tmp->v; else for(tmp=list;tmp!=NULL;tmp=tmp->next) out[i++]=tmp->v; } /* Return the created array. */ return out; } void gal_list_f64_free(gal_list_f64_t *list) { gal_list_f64_t *tmp, *ttmp; tmp=list; while(tmp!=NULL) { ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** ***************** void * ******************** ****************************************************************/ void gal_list_void_add(gal_list_void_t **list, void *value) { gal_list_void_t *newnode; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->next=*list; *list=newnode; } void * gal_list_void_pop(gal_list_void_t **list) { void *out=NULL; gal_list_void_t *tmp; if(*list) { tmp=*list; out=tmp->v; *list=tmp->next; free(tmp); } return out; } size_t gal_list_void_number(gal_list_void_t *list) { size_t num=0; gal_list_void_t *tmp; for(tmp=list;tmp!=NULL;tmp=tmp->next) ++num; return num; } void gal_list_void_reverse(gal_list_void_t **list) { void *thisptr; gal_list_void_t *correctorder=NULL; if( *list && (*list)->next ) { while(*list!=NULL) { thisptr=gal_list_void_pop(list); gal_list_void_add(&correctorder, thisptr); } *list=correctorder; } } void gal_list_void_free(gal_list_void_t *list, int freevalue) { gal_list_void_t *tmp=list, *ttmp; while(tmp!=NULL) { if(freevalue) free(tmp->v); ttmp=tmp->next; free(tmp); tmp=ttmp; } } /**************************************************************** **************** Ordered size_t ******************** ****************************************************************/ /* We want to put the nodes in order based on the 'tosort' value of each node. The top element should always have the smallest radius. */ void gal_list_osizet_add(gal_list_osizet_t **list, size_t value, float tosort) { gal_list_osizet_t *newnode, *tmp=*list, *prev=NULL; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->s=tosort; /* *list points to the smallest value in the queue!*/ while(tmp!=NULL) { if(tosorts) break; /* No need for else, it will only come here if the condition above is not satisfied. */ prev=tmp; tmp=tmp->next; } if(tmp==NULL) /* This is the largest value so far. */ { /* '*list' only changes if it is NULL. */ newnode->next=NULL; if(prev) prev->next=newnode; /* 'prev' is not NULL! */ else *list=newnode; /* Only for initial node. */ } else { if(prev) prev->next=newnode; else *list=newnode; /* 'tosort' is smaller than all. */ newnode->next=tmp; } } /* Note that the popped element is the smallest! */ size_t gal_list_osizet_pop(gal_list_osizet_t **list, float *sortvalue) { size_t value; gal_list_osizet_t *tmp=*list; if(*list) { value=tmp->v; *sortvalue=tmp->s; *list=tmp->next; free(tmp); } else { value=GAL_BLANK_SIZE_T; *sortvalue=NAN; } return value; } /* Add the elements of an gal_list_osll to a gal_list_sll. */ void gal_list_osizet_to_sizet_free(gal_list_osizet_t *in, gal_list_sizet_t **out) { gal_list_osizet_t *tmp; while(in!=NULL) { tmp=in->next; gal_list_sizet_add(out, in->v); free(in); in=tmp; } } /**************************************************************** ****************** Two way, Ordered SLL ******************** ***************** size_t ******************** ****************************************************************/ /* Doubly-linked ordered size_t list can be visualized like this: largest pointer | NULL <-- (v0,s0) <--> (v1,s1) <--> ... (vn,sn) --> NULL | smallest pointer Where s(n)>s(n+1) for all n. */ /* Very similar to Ordered SLL, but now it is two way. */ void gal_list_dosizet_add(gal_list_dosizet_t **largest, gal_list_dosizet_t **smallest, size_t value, float tosort) { gal_list_dosizet_t *newnode, *tmp=*largest; errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->v=value; newnode->s=tosort; newnode->prev=NULL; while(tmp!=NULL) { if(tosort >= tmp->s) break; /* No need for else, it will only come here if the condition above is not satisfied. */ newnode->prev=tmp; tmp=tmp->next; } if(tmp==NULL) /* This is the smallest value so far. */ { /* '*largest' only changes if it is NULL. */ newnode->next=NULL; *smallest=newnode; if(newnode->prev) /* 'prev' is not NULL! */ newnode->prev->next=newnode; else /* 'prev is NULL, Only first. */ *largest=newnode; } else { if(newnode->prev) { newnode->prev->next->prev=newnode; newnode->prev->next=newnode; } else { (*largest)->prev=newnode; *largest=newnode; /* 'tosort' is larger than all. */ } newnode->next=tmp; } } /* Note that start has to be initialized. */ size_t gal_list_dosizet_pop_smallest(gal_list_dosizet_t **largest, gal_list_dosizet_t **smallest, float *tosort) { size_t value; gal_list_dosizet_t *tmp=*smallest; if(*smallest) { value=tmp->v; *tosort=tmp->s; *smallest=tmp->prev; free(tmp); if(*smallest) (*smallest)->next=NULL; else *largest=NULL; } else { /* If `smallest' is NULL, `largest' should also be NULL. */ if(*largest) error(EXIT_FAILURE, 0, "%s: `largest' and `smallest' pointers must " "both be non-NULL or both be NULL. However, in this call, " "`smallest' was NULL while `largest' isn't NULL", __func__); value=GAL_BLANK_SIZE_T; *tosort=NAN; } /*printf("Popped v: %zu, s: %f\n", *value, *tosort);*/ return value; } void gal_list_dosizet_print(gal_list_dosizet_t *largest, gal_list_dosizet_t *smallest) { size_t counter=1; /* We are not counting array elements :-D ! */ while(largest!=NULL) { printf("\t%-5zu (%zu, %.4f) \n", counter++, largest->v, largest->s); largest=largest->next; printf("\t\t\t\t(%zu, %.4f)\n", smallest->v, smallest->s); smallest=smallest->prev; } printf("\n"); } void gal_list_dosizet_to_sizet(gal_list_dosizet_t *in, gal_list_sizet_t **out) { gal_list_dosizet_t *tmp; while(in!=NULL) { tmp=in->next; gal_list_sizet_add(out, in->v); free(in); in=tmp; } } void gal_list_dosizet_free(gal_list_dosizet_t *largest) { gal_list_dosizet_t *tmp; while(largest!=NULL) { tmp=largest->next; free(largest); largest=tmp; } } /*********************************************************************/ /************* Data structure as a linked list ******************/ /*********************************************************************/ /* Add a new data structure to the top of an existing linked list of data structures. Note that if the new node is its self a list, all its nodes will be added to the list. */ void gal_list_data_add(gal_data_t **list, gal_data_t *newnode) { gal_data_t *tmp=newnode, *toadd; /* Check if newnode is itself a list or not. */ if(newnode->next) { /* Go onto the last node in newnode's existing list. */ while(tmp->next) tmp=tmp->next; /* Set the last node as the node to add to the list. */ toadd=tmp; } else /* Its not a list, so just set it to `toadd'. */ toadd=newnode; /* Set the next element of toadd and update what list points to.*/ toadd->next=*list; *list=toadd; } void gal_list_data_add_alloc(gal_data_t **list, void *array, uint8_t type, size_t ndim, size_t *dsize, struct wcsprm *wcs, int clear, size_t minmapsize, char *name, char *unit, char *comment) { gal_data_t *newnode; /* Put all the input information into a new data structure node. */ newnode=gal_data_alloc(array, type, ndim, dsize, wcs, clear, minmapsize, name, unit, comment); /* Add the new node to the list. */ gal_list_data_add(list, newnode); } gal_data_t * gal_list_data_pop(gal_data_t **list) { gal_data_t *out=NULL; /* If list is not empty. */ if(*list) { /* Keep the top pointer. */ out=*list; /* Move the list pointer to the next node. */ *list=out->next; /* Set the next poitner of the out pointer to NULL so it isn't interpretted as a list any more. */ out->next=NULL; } return out; } void gal_list_data_reverse(gal_data_t **list) { gal_data_t *popped, *in=*list, *reversed=NULL; /* Only do the job if the list is not NULL and has more than one node. */ if( in && in->next ) { while(in!=NULL) { popped=gal_list_data_pop(&in); gal_list_data_add(&reversed, popped); } *list=reversed; } } size_t gal_list_data_number(gal_data_t *list) { size_t num=0; while(list!=NULL) { ++num; list=list->next; } return num; } void gal_list_data_free(gal_data_t *list) { struct gal_data_t *tmp; while(list!=NULL) { tmp=list->next; gal_data_free(list); list=tmp; } } gnuastro-0.5/lib/interpolate.c0000644000175000017500000003662313121462410013405 00000000000000/********************************************************************* Interpolate - Fill blank values in a dataset This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /*********************************************************************/ /******************** Nearest neighbor ********************/ /*********************************************************************/ /* These are bit-flags, so we're using hexadecimal notation. */ #define INTERPOLATE_FLAGS_NO 0 #define INTERPOLATE_FLAGS_CHECKED 0x1 #define INTERPOLATE_FLAGS_BLANK 0x2 /* Parameters for interpolation on threads. */ struct interpolate_params { gal_data_t *input; size_t num; gal_data_t *out; gal_data_t *blanks; size_t numneighbors; uint8_t *thread_flags; int onlyblank; gal_list_void_t *ngb_vals; struct gal_tile_two_layer_params *tl; }; /* Run the interpolation on many threads. */ static void * interpolate_close_neighbors_on_thread(void *in_prm) { /* Variables that others depend on. */ struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct interpolate_params *prm=(struct interpolate_params *)(tprm->params); struct gal_tile_two_layer_params *tl=prm->tl; int correct_index=(tl && tl->totchannels>1 && !tl->workoverch); gal_data_t *input=prm->input; /* Rest of variables. */ void *nv; float pdist; uint8_t *b, *bf, *bb; gal_list_void_t *tvll; gal_list_dosizet_t *lQ, *sQ; size_t ngb_counter, dist, pind, *dinc; size_t i, index, fullind, chstart=0, ndim=input->ndim; gal_data_t *median, *tin, *tout, *tnear, *nearest=NULL; size_t *icoord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "icoord"); size_t *ncoord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "ncoord"); size_t size = (correct_index ? tl->tottilesinch : input->size); size_t *dsize = (correct_index ? tl->numtilesinch : input->dsize); uint8_t *fullflag=&prm->thread_flags[tprm->id*input->size], *flag=fullflag; /* Initializations. */ bb=prm->blanks->array; bf=(b=fullflag)+input->size; dinc=gal_dimension_increment(ndim, dsize); do *b = *bb++ ? INTERPOLATE_FLAGS_BLANK : 0; while(++bngb_vals; tvll!=NULL; tvll=tvll->next) { nv=gal_data_ptr_increment(tvll->v, tprm->id*prm->numneighbors, input->type); gal_list_data_add_alloc(&nearest, nv, tin->type, 1, &prm->numneighbors, NULL, 0, -1, NULL, NULL, NULL); tin=tin->next; } gal_list_data_reverse(&nearest); /* Go over all the points given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* For easy reading. */ fullind=tprm->indexs[i]; /* If the caller only wanted to interpolate over blank values and this value is not blank (we know from the flags), then just set the output value at this element to the input value and go to the next element. */ if(prm->onlyblank && !(fullflag[fullind] & INTERPOLATE_FLAGS_BLANK) ) { tin=input; for(tout=prm->out; tout!=NULL; tout=tout->next) { memcpy(gal_data_ptr_increment(tout->array, fullind, tin->type), gal_data_ptr_increment(tin->array, fullind, tin->type), gal_type_sizeof(tin->type)); tin=tin->next; } continue; } /* Correct the index (if necessary). When the values come from a tiled dataset, the caller might want to interpolate the values of each channel separately (not mix values from different channels). In such a case, the tiles of each channel (and their values in `input' are contiguous. So we need to correct `tprm->indexs[i]' (which is the index over the whole tessellation, including all channels). */ if(correct_index) { /* Index of this tile in its channel. */ index = fullind % tl->tottilesinch; /* Index of the first tile in this channel. */ chstart = (fullind / tl->tottilesinch) * tl->tottilesinch; /* Set the channel's starting pointer for the flags. */ flag = gal_data_ptr_increment(fullflag, chstart, GAL_TYPE_UINT8); } else { chstart=0; index=fullind; } /* Reset all checked bits in the flags array to 0. */ ngb_counter=0; bf=(b=flag)+size; do *b &= ~(INTERPOLATE_FLAGS_CHECKED); while(++bnext) { memcpy(gal_data_ptr_increment(tnear->array, ngb_counter, tin->type), gal_data_ptr_increment(tin->array, chstart+pind, tin->type), gal_type_sizeof(tin->type)); tin=tin->next; } /* If we have filled all the elements clean up the linked list and break out. */ if(++ngb_counter>=prm->numneighbors) { if(lQ) gal_list_dosizet_free(lQ); break; } } /* Go over all the neighbors of this popped pixel and add them to the list of neighbors to be checked. */ GAL_DIMENSION_NEIGHBOR_OP(pind, ndim, dsize, 1, dinc, { /* Only look at neighbors that have not been checked. VERY IMPORTANT: we must not check for blank values here, otherwise we won't be able to parse over extended blank regions. */ if( !(flag[nind] & INTERPOLATE_FLAGS_CHECKED) ) { /* Get the coordinates of this neighbor. */ gal_dimension_index_to_coord(nind, ndim, dsize, ncoord); /* Distance of this neighbor to the one to be filled. */ dist=gal_dimension_dist_manhattan(icoord, ncoord, ndim); /* Add this neighbor to the list. */ gal_list_dosizet_add(&lQ, &sQ, nind, dist); /* Flag this neighbor as checked. */ flag[nind] |= INTERPOLATE_FLAGS_CHECKED; } } ); /* If there are no more meshes to add to the queue, then this shows, there were not enough points for interpolation. Normally, this loop should only be exited through the `currentnum>=numnearest' check above. */ if(sQ==NULL) error(EXIT_FAILURE, 0, "%s: only %zu neighbors found while " "you had asked to use %zu neighbors for close neighbor " "interpolation", __func__, ngb_counter, prm->numneighbors); } /* Calculate the median of the values and write it in the output. */ tout=prm->out; for(tnear=nearest; tnear!=NULL; tnear=tnear->next) { /* Find the median and copy it. */ median=gal_statistics_median(tnear, 1); memcpy(gal_data_ptr_increment(tout->array, fullind, tout->type), median->array, gal_type_sizeof(tout->type)); /* Clean up and go to next array. */ gal_data_free(median); tout=tout->next; } } /* Clean up. */ for(tnear=nearest; tnear!=NULL; tnear=tnear->next) tnear->array=NULL; gal_list_data_free(nearest); free(icoord); free(ncoord); free(dinc); /* Wait for all the other threads to finish and return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* When no interpolation is needed, then we can just copy the input into the output. */ static gal_data_t * interpolate_copy_input(gal_data_t *input, int aslinkedlist) { gal_data_t *tin, *tout; /* Make a copy of the first input. */ tout=gal_data_copy(input); tout->next=NULL; /* If we have a linked list, copy each element. */ if(aslinkedlist) { /* Note that we have already copied the first input. */ for(tin=input->next; tin!=NULL; tin=tin->next) { /* Copy this dataset (will also copy flags). */ tout->next=gal_data_copy(tin); tout=tout->next; } /* Output is the reverse of the input, so reverse it. */ gal_list_data_reverse(&tout); } /* Return the copied list. */ return tout; } /* Interpolate blank values in an array. If the `tl!=NULL', then it is assumed that the tile values correspond to given tessellation. Such that `input[i]' corresponds to `tiles[i]' in the tessellation. */ gal_data_t * gal_interpolate_close_neighbors(gal_data_t *input, struct gal_tile_two_layer_params *tl, size_t numneighbors, size_t numthreads, int onlyblank, int aslinkedlist) { gal_data_t *tin, *tout; struct interpolate_params prm; size_t ngbvnum=numthreads*numneighbors; int permute=(tl && tl->totchannels>1 && tl->workoverch); /* If there are no blank values in the array we should only fill blank values, then simply copy the input and abort. */ if( (input->flag | GAL_DATA_FLAG_BLANK_CH) /* Zero bit is meaningful.*/ && !(input->flag | GAL_DATA_FLAG_HASBLANK) /* There are no blanks. */ && onlyblank ) /* Only interpolate blank.*/ return interpolate_copy_input(input, aslinkedlist); /* Initialize the constant parameters. */ prm.tl = tl; prm.ngb_vals = NULL; prm.input = input; prm.onlyblank = onlyblank; prm.numneighbors = numneighbors; prm.num = aslinkedlist ? gal_list_data_number(input) : 1; /* Flag the blank values. */ prm.blanks=gal_blank_flag(input); /* If the input is from a tile structure and the user has asked to ignore channels, then re-order the values. */ if(permute) { /* Prepare the permutation (if necessary/not already defined). */ gal_tile_full_permutation(tl); /* Re-order values to ignore channels (if necessary). */ gal_permutation_apply(input, tl->permutation); gal_permutation_apply(prm.blanks, tl->permutation); /* If this is a linked list, then permute remaining nodes. */ if(aslinkedlist) for(tin=input->next; tin!=NULL; tin=tin->next) gal_permutation_apply(tin, tl->permutation); } /* Allocate space for the (first) output. */ prm.out=gal_data_alloc(NULL, input->type, input->ndim, input->dsize, input->wcs, 0, input->minmapsize, NULL, input->unit, NULL); gal_list_void_add(&prm.ngb_vals, gal_data_malloc_array(input->type, ngbvnum, __func__, "prm.ngb_vals")); /* If we are given a list of datasets, make the necessary allocations. The reason we are doing this after a check of `aslinkedlist' is that the `input' might have a `next' element, but the caller might not have called `aslinkedlist'. */ prm.out->next=NULL; if(aslinkedlist) for(tin=input->next; tin!=NULL; tin=tin->next) { /* A small sanity check. */ if( gal_data_dsize_is_different(input, tin) ) error(EXIT_FAILURE, 0, "%s: all datasets in the list must have " "the same dimension and size", __func__); /* Allocate the output array for this node. */ gal_list_data_add_alloc(&prm.out, NULL, tin->type, tin->ndim, tin->dsize, tin->wcs, 0, tin->minmapsize, NULL, tin->unit, NULL); /* Allocate the space for the neighbor values of this input. */ gal_list_void_add(&prm.ngb_vals, gal_data_malloc_array(tin->type, ngbvnum, __func__, "prm.ngb_vals")); } gal_list_data_reverse(&prm.out); gal_list_void_reverse(&prm.ngb_vals); /* Allocate space for all the flag values of all the threads here (memory in each thread is limited) and this is cleaner. */ prm.thread_flags=gal_data_malloc_array(GAL_TYPE_UINT8, numthreads*input->size, __func__, "prm.thread_flags"); /* Spin off the threads. */ gal_threads_spin_off(interpolate_close_neighbors_on_thread, &prm, input->size, numthreads); /* If the values were permuted for the interpolation, then re-order the values back to their original location (so they correspond to their tile indexs. */ if(permute) { gal_permutation_apply_inverse(input, tl->permutation); for(tout=prm.out; tout!=NULL; tout=tout->next) gal_permutation_apply_inverse(tout, tl->permutation); } /* The interpolated array doesn't have blank values. So set the blank flag to 0 and set the use-zero to 1. */ for(tout=prm.out; tout!=NULL; tout=tout->next) { tout->flag |= GAL_DATA_FLAG_BLANK_CH; tout->flag &= ~GAL_DATA_FLAG_HASBLANK; } /* Clean up and return. */ free(prm.thread_flags); gal_data_free(prm.blanks); gal_list_void_free(prm.ngb_vals, 1); return prm.out; } gnuastro-0.5/lib/git.c0000644000175000017500000000475313121462410011641 00000000000000/********************************************************************* Functions to deal with Git version controlled directories. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include /* Return the result of Git describe and */ char * gal_git_describe(void) { char *describe_return=NULL; /* Only actually work on Git if the library is present. */ #if GAL_CONFIG_HAVE_LIBGIT2 == 1 git_buf buf={0}; git_repository *repo; git_describe_result *describe_result; git_describe_format_options format_options; git_describe_options describe_options = GIT_DESCRIBE_OPTIONS_INIT; /* Initialize Git's global setup. */ git_libgit2_init(); /* Initialize the descriptions. */ git_describe_init_format_options(&format_options, GIT_DESCRIBE_FORMAT_OPTIONS_VERSION); /* Set some values manually: */ describe_options.show_commit_oid_as_fallback=1; format_options.dirty_suffix="-dirty"; /* Open the Git repository. */ if( !git_repository_open_ext(&repo, ".", 0, NULL) && !git_describe_workdir(&describe_result, repo, &describe_options) && !git_describe_format(&buf, describe_result, &format_options) ) { /* Allocate space for and copy the description. */ errno=0; describe_return=malloc(strlen(buf.ptr)+1); if(describe_return==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes to copy " "Git's describe", __func__, strlen(buf.ptr)+1); strcpy(describe_return, buf.ptr); } /* Clean up. */ git_repository_free(repo); git_libgit2_shutdown(); #endif /* Return */ return describe_return; } gnuastro-0.5/lib/fits.c0000644000175000017500000025250513211076737012040 00000000000000/********************************************************************* Functions to work with FITS image data. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /************************************************************* ************** Reporting errors: *************** *************************************************************/ void gal_fits_io_error(int status, char *message) { char defmessage[]="Error in CFITSIO, see above."; if(status) { fits_report_error(stderr, status); if(message) error(EXIT_FAILURE, 0, "%s", message); else error(EXIT_FAILURE, 0, "%s", defmessage); } } /************************************************************* ************** FITS names *************** *************************************************************/ /* IMPORTANT NOTE: if other compression suffixes are add to this function, include them in `gal_checkset_automatic_output', so the compression suffix can be skipped when the user doesn't specify an output filename.*/ int gal_fits_name_is_fits(char *name) { size_t len; len=strlen(name); if ( ( len>=3 && strcmp(&name[len-3], "fit" ) == 0 ) || ( len>=4 && strcmp(&name[len-4], "fits" ) == 0 ) || ( len>=7 && strcmp(&name[len-7], "fits.gz" ) == 0 ) || ( len>=6 && strcmp(&name[len-6], "fits.Z" ) == 0 ) || ( len>=3 && strcmp(&name[len-3], "imh" ) == 0 ) || ( len>=7 && strcmp(&name[len-7], "fits.fz" ) == 0 ) ) return 1; else return 0; } /* IMPORTANT NOTE: if other compression suffixes are add to this function, include them in `gal_checkset_automatic_output', so the compression suffix can be skipped when the user doesn't specify an output filename.*/ int gal_fits_suffix_is_fits(char *suffix) { char *nodot = suffix[0]=='.' ? (suffix+1) : suffix; if ( strcmp( nodot, "fit" ) == 0 || strcmp(nodot, "fits" ) == 0 || strcmp(nodot, "fits.gz" ) == 0 || strcmp(nodot, "fits.Z" ) == 0 || strcmp(nodot, "imh" ) == 0 || strcmp(nodot, "fits.fz" ) == 0 ) return 1; else return 0; } /* If the name is a FITS name, then put a `(hdu: ...)' after it and return the string. If it isn't a FITS file, just print the name. Note that the space is allocated. */ char * gal_fits_name_save_as_string(char *filename, char *hdu) { char *name; if( gal_fits_name_is_fits(filename) ) asprintf(&name, "%s (hdu: %s)", filename, hdu); else gal_checkset_allocate_copy(filename, &name); return name; } /************************************************************* ************** Type codes *************** *************************************************************/ uint8_t gal_fits_bitpix_to_type(int bitpix) { switch(bitpix) { case BYTE_IMG: return GAL_TYPE_UINT8; case SBYTE_IMG: return GAL_TYPE_INT8; case USHORT_IMG: return GAL_TYPE_UINT16; case SHORT_IMG: return GAL_TYPE_INT16; case ULONG_IMG: return GAL_TYPE_UINT32; case LONG_IMG: return GAL_TYPE_INT32; case LONGLONG_IMG: return GAL_TYPE_INT64; case FLOAT_IMG: return GAL_TYPE_FLOAT32; case DOUBLE_IMG: return GAL_TYPE_FLOAT64; default: error(EXIT_FAILURE, 0, "%s: bitpix value of %d not recognized", __func__, bitpix); } return 0; } int gal_fits_type_to_bitpix(uint8_t type) { switch(type) { case GAL_TYPE_UINT8: return BYTE_IMG; case GAL_TYPE_INT8: return SBYTE_IMG; case GAL_TYPE_UINT16: return USHORT_IMG; case GAL_TYPE_INT16: return SHORT_IMG; case GAL_TYPE_UINT32: return ULONG_IMG; case GAL_TYPE_INT32: return LONG_IMG; case GAL_TYPE_INT64: return LONGLONG_IMG; case GAL_TYPE_FLOAT32: return FLOAT_IMG; case GAL_TYPE_FLOAT64: return DOUBLE_IMG; case GAL_TYPE_BIT: case GAL_TYPE_STRLL: case GAL_TYPE_STRING: case GAL_TYPE_UINT64: case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: error(EXIT_FAILURE, 0, "%s: type %s not recognized for FITS image " "BITPIX", __func__, gal_type_name(type, 1)); default: error(EXIT_FAILURE, 0, "%s: type value of %d not recognized", __func__, type); } return 0; } /* The values to the TFORM header keywords of FITS binary tables are single letter capital letters, but that is useless in identifying the data type of the column. So this function will do the conversion based on the CFITSIO manual.*/ char gal_fits_type_to_bin_tform(uint8_t type) { switch(type) { /* Recognized by CFITSIO. */ case GAL_TYPE_STRING: return 'A'; case GAL_TYPE_BIT: return 'X'; case GAL_TYPE_UINT8: return 'B'; case GAL_TYPE_INT8: return 'S'; case GAL_TYPE_UINT16: return 'U'; case GAL_TYPE_INT16: return 'I'; case GAL_TYPE_UINT32: return 'V'; case GAL_TYPE_INT32: return 'J'; case GAL_TYPE_INT64: return 'K'; case GAL_TYPE_FLOAT32: return 'E'; case GAL_TYPE_FLOAT64: return 'D'; case GAL_TYPE_COMPLEX32: return 'C'; case GAL_TYPE_COMPLEX64: return 'M'; /* Not recognized by CFITSIO. */ case GAL_TYPE_UINT64: error(EXIT_FAILURE, 0, "%s: type %s not recognized for FITS binary " "table TFORM", __func__, gal_type_name(type, 1)); break; /* Wrong type code. */ default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } error(EXIT_FAILURE, 0, "%s: s bug! Please contact us so we can fix this. " "Control must not reach the end of this function", __func__); return '\0'; } int gal_fits_type_to_datatype(uint8_t type) { int w=0; switch(type) { /* Recognized CFITSIO types. */ case GAL_TYPE_BIT: return TBIT; case GAL_TYPE_UINT8: return TBYTE; case GAL_TYPE_INT8: return TSBYTE; case GAL_TYPE_FLOAT32: return TFLOAT; case GAL_TYPE_FLOAT64: return TDOUBLE; case GAL_TYPE_COMPLEX32: return TCOMPLEX; case GAL_TYPE_COMPLEX64: return TDBLCOMPLEX; case GAL_TYPE_STRING: return TSTRING; /* Types that depend on the host system. The C standard says that the `short', `int' and `long' types are ATLEAST 2, 2, 4 bytes, so be safe, we will checking all of them for the 32-bit types.*/ case GAL_TYPE_UINT16: w=2; if ( sizeof(short) == w ) return TUSHORT; else if( sizeof(int) == w ) return TUINT; break; case GAL_TYPE_INT16: w=2; if ( sizeof(short) == w ) return TSHORT; else if( sizeof(int) == w ) return TINT; break; /* On 32-bit systems, the length of `int' and `long' are both 32-bits. But CFITSIO's LONG type is preferred because it is designed to be 32-bit. Its `INT' type is not clearly defined and caused problems when reading keywords.*/ case GAL_TYPE_UINT32: w=4; if ( sizeof(long) == w ) return TULONG; else if( sizeof(int) == w ) return TUINT; else if( sizeof(short) == w ) return TUSHORT; break; /* Similar to UINT32 above. */ case GAL_TYPE_INT32: w=4; if ( sizeof(long) == w ) return TLONG; else if( sizeof(int) == w ) return TINT; else if( sizeof(short) == w ) return TSHORT; break; case GAL_TYPE_UINT64: w=8; if ( sizeof(long) == w ) return TULONG; break; case GAL_TYPE_INT64: w=8; if ( sizeof(long) == w ) return TLONG; else if( sizeof(LONGLONG) == w ) return TLONGLONG; break; /* Wrong type. */ default: error(EXIT_FAILURE, 0, "%s: type code %d is not a recognized", __func__, type); } /* If control reaches, here, there was a problem with the host types. */ if(w) error(EXIT_FAILURE, 0, "%s: this system doesn't have a %d byte integer " "type, so type `%s' cannot be written to FITS", __func__, w, gal_type_name(type, 1)); else error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "fix the problem. Control must not have reached the end for the " "given type `%s'", __func__, PACKAGE_BUGREPORT, gal_type_name(type, 1)); return -1; } uint8_t gal_fits_datatype_to_type(int datatype, int is_table_column) { int inttype; switch(datatype) { case TBIT: return GAL_TYPE_BIT; case TBYTE: return GAL_TYPE_UINT8; case TSBYTE: return GAL_TYPE_INT8; case TFLOAT: return GAL_TYPE_FLOAT32; case TDOUBLE: return GAL_TYPE_FLOAT64; case TCOMPLEX: return GAL_TYPE_COMPLEX32; case TDBLCOMPLEX: return GAL_TYPE_COMPLEX64; case TSTRING: return GAL_TYPE_STRING; /* Sizes that depend on the host system. */ case TUSHORT: switch( sizeof(short) ) { case 2: return GAL_TYPE_UINT16; case 4: return GAL_TYPE_UINT32; case 8: return GAL_TYPE_UINT64; } break; case TSHORT: switch( sizeof(short) ) { case 2: return GAL_TYPE_INT16; case 4: return GAL_TYPE_INT32; case 8: return GAL_TYPE_INT64; } break; case TUINT: switch( sizeof(int) ) { case 2: return GAL_TYPE_UINT16; case 4: return GAL_TYPE_UINT32; case 8: return GAL_TYPE_UINT64; } break; case TINT: switch( sizeof(int) ) { case 2: return GAL_TYPE_INT16; case 4: return GAL_TYPE_INT32; case 8: return GAL_TYPE_INT64; } break; case TULONG: switch( sizeof(long) ) { case 4: return GAL_TYPE_UINT32; case 8: return GAL_TYPE_UINT64; } break; case TLONG: /* ==TINT32BIT when in a table column. */ if(is_table_column) return GAL_TYPE_INT32; else switch( sizeof(long) ) { case 4: return GAL_TYPE_INT32; case 8: return GAL_TYPE_INT64; } break; case TLONGLONG: return GAL_TYPE_INT64; break; /* The TLOGICAL depends on the context: for keywords, it is int32, for table columns, it is int8. */ case TLOGICAL: switch( sizeof(int) ) { case 2: inttype=GAL_TYPE_INT16; break; case 4: inttype=GAL_TYPE_INT32; break; case 8: inttype=GAL_TYPE_INT64; break; } return is_table_column ? GAL_TYPE_INT8 : inttype; break; /* A bug! */ default: error(EXIT_FAILURE, 0, "%s: %d is not a recognized CFITSIO datatype", __func__, datatype); } error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can fix " "this. Control must not have reached the end of this function.", __func__, PACKAGE_BUGREPORT); return GAL_TYPE_INVALID; } /* When there is a BZERO or TZERO and BSCALE or TSCALE keywords, then the type that must be used to store the actual values of the pixels may be different from the type from BITPIX. This function does the necessary corrections.*/ static void fits_type_correct(int *type, double bscale, char *bzero_str) { double bzero; int tofloat=1; char *tailptr, *bzero_u64="9223372036854775808"; /* If bzero_str is given and `bscale=1.0' the case might be that we are dealing with an integer dataset that just needs a different sign. */ if(bzero_str && bscale==1.0f) { /* Read the `bzero' string as a `double' number. */ bzero = strtod(bzero_str, &tailptr); if(tailptr==bzero_str) error(EXIT_FAILURE, 0, "%s: BZERO value `%s' couldn't be " "parsed as a number", __func__, bzero_str); /* Work based on type. For the default conversions defined by the FITS standard to change the signs of integers, make the proper correction, otherwise set the type to float. */ switch(*type) { case GAL_TYPE_UINT8: if(bzero == -128.0f) { *type = GAL_TYPE_INT8; tofloat=0; } break; case GAL_TYPE_INT16: if(bzero == 32768) { *type = GAL_TYPE_UINT16; tofloat=0; } break; case GAL_TYPE_INT32: if(bzero == 2147483648LU) { *type = GAL_TYPE_UINT32; tofloat=0; } break; /* The `bzero' value for unsigned 64-bit integers has 19 decimal digits, but a 64-bit floating point (`double' type) can only safely store 15 decimal digits. As a result, the safest way to check the `bzero' value for this type is to compare it as a string. But all integers nearby (for example `9223372036854775807') get rounded to this same value (when stored as `double'). So we will also check the parsed number and if it equals this number, a warning will be printed. */ case GAL_TYPE_INT64: if( !strcmp(bzero_str, bzero_u64) ) {*type = GAL_TYPE_UINT64; tofloat=0;} else if( bzero == 9223372036854775808LLU ) { fprintf(stderr, "\nWARNING in %s: the BZERO header keyword " "value (`%s') is very close (but not exactly equal) " "to `%s'. The latter value in the FITS standard is " "used to identify that the dataset should be read as " "unsigned 64-bit integers instead of signed 64-bit " "integers. Depending on your version of CFITSIO, " "it may be read as a signed or unsigned 64-bit " "integer array\n\n", __func__, bzero_str, bzero_u64); tofloat=0; } break; /* For the other types (when `BSCALE=1.0f'), currently no correction is necessary, maybe later we can check if the scales are integers and set the integer output type to the smallest type that can allow the scaled values. */ default: tofloat=0; } } /* If the type must be a float, then do the conversion. */ if(tofloat) *type=GAL_TYPE_FLOAT32; } /**************************************************************/ /********** HDU ************/ /**************************************************************/ fitsfile * gal_fits_open_to_write(char *filename) { int status=0; long naxes=0; fitsfile *fptr; /* When the file exists just open it. Otherwise, create the file. But we want to leave the first extension as a blank extension and put the image in the next extension to be consistent between tables and images. */ if(access(filename,F_OK) == -1 ) { /* Create the file. */ if( fits_create_file(&fptr, filename, &status) ) gal_fits_io_error(status, NULL); /* Create blank extension. */ if( fits_create_img(fptr, BYTE_IMG, 0, &naxes, &status) ) gal_fits_io_error(status, NULL); /* Close the blank extension. */ if( fits_close_file(fptr, &status) ) gal_fits_io_error(status, NULL); } /* Open the file, ready for later steps. */ if( fits_open_file(&fptr, filename, READWRITE, &status) ) gal_fits_io_error(status, NULL); /* Return the pointer. */ return fptr; } size_t gal_fits_hdu_num(char *filename) { fitsfile *fptr; int num, status=0; /* We don't need to check for an error everytime, because we don't make any non CFITSIO usage of the output. It is necessary to check every CFITSIO call, only when you will need to use the outputs. */ fits_open_file(&fptr, filename, READONLY, &status); fits_get_num_hdus(fptr, &num, &status); fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); return num; } /* Given the filename and HDU, this function will return the CFITSIO code for the type of data it contains (table, or image). The CFITSIO codes are: IMAGE_HDU: An image HDU. ASCII_TBL: An ASCII table HDU. BINARY_TBL: BINARY TABLE HDU. */ int gal_fits_hdu_format(char *filename, char *hdu) { fitsfile *fptr; int hdutype, status=0; /* Open the HDU. */ fptr=gal_fits_hdu_open(filename, hdu, READONLY); /* Check the type of the given HDU: */ if (fits_get_hdu_type(fptr, &hdutype, &status) ) gal_fits_io_error(status, NULL); /* Clean up and return.. */ if( fits_close_file(fptr, &status) ) gal_fits_io_error(status, NULL); return hdutype; } /* Open a given HDU and return the FITS pointer. `iomode' determines how the FITS file will be opened: only to read or to read and write. You should use the macros given by the CFITSIO header: READONLY: read-only. READWRITE: read and write. */ fitsfile * gal_fits_hdu_open(char *filename, char *hdu, int iomode) { int status=0; char *ffname; fitsfile *fptr; /* Add hdu to filename: */ asprintf(&ffname, "%s[%s#]", filename, hdu); /* Open the FITS file: */ if( fits_open_file(&fptr, ffname, iomode, &status) ) { switch(status) { /* Since the default HDU is `1', when the file only has one extension, this error is common, so we will put a special notice. */ case END_OF_FILE: if( hdu[0]=='1' && hdu[1]=='\0' ) error(EXIT_FAILURE, 0, "%s has only one extension/HDU but you " "have asked for the second HDU (hdu number 1 in CFITSIO)." "\n\n" "To fix the problem please add `--hdu=0' (or `-h0') to " "your command when calling Gnuastro's programs. For " "library users, please give a value of \"0\" to the HDU " "argument.\n\n" "FOOTNOTE -- When writing a new FITS file, Gnuastro leaves " "the first HDU blank (with no data) and writes the " "outputs in the second HDU. In this way the keywords of " "the the first HDU can be used as meta data of the whole " "file (which may contain many extensions). This is the " "recommended way in the FITS standard. As a result, " "Gnuastro's default HDU to read an extension in a FITS " "file is the second. This error is commonly caused when " "the FITS file wasn't created according to this " "convention.", filename); break; /* Generic error below is fine for this case */ case BAD_HDU_NUM: break; /* In case an un-expected error occurs, use the general CFITSIO reporting that we have already prepared. */ default: gal_fits_io_error(status, "opening the given extension/HDU in " "the given file"); } error(EXIT_FAILURE, 0, "%s: extension/HDU `%s' doesn't exist. Please " "run the following command to see the extensions/HDUs in " "`%s':\n\n" " $ astfits %s\n\n" "The respective HDU number (or name, when present) may be used " "with the `--hdu' option in Gnuastro's programs (or the `hdu' " "argument in Gnuastro's libraries) to open the respective HDU.", filename, hdu, filename, filename); } /* Clean up and the pointer. */ free(ffname); return fptr; } /* Check the desired HDU in a FITS image and also if it has the desired type. */ fitsfile * gal_fits_hdu_open_format(char *filename, char *hdu, int img0_tab1) { fitsfile *fptr; int status=0, hdutype; /* A small sanity check. */ if(hdu==NULL) error(EXIT_FAILURE, 0, "no HDU specified for %s", filename); /* Open the HDU. */ fptr=gal_fits_hdu_open(filename, hdu, READONLY); /* Check the type of the given HDU: */ if (fits_get_hdu_type(fptr, &hdutype, &status) ) gal_fits_io_error(status, NULL); /* Check if the type of the HDU is the expected type. We could have written these as && conditions, but this is easier to read, it makes no meaningful difference to the compiler. */ if(img0_tab1) { if(hdutype==IMAGE_HDU) error(EXIT_FAILURE, 0, "%s (hdu: %s): is not a table", filename, hdu); } else { if(hdutype!=IMAGE_HDU) error(EXIT_FAILURE, 0, "%s (hdu: %s): not an image", filename, hdu); } /* Clean up and return. */ return fptr; } /**************************************************************/ /********** Header keywords ************/ /**************************************************************/ /* Return allocated pointer to the blank value to use in a FITS file header keyword. */ void * gal_fits_key_img_blank(uint8_t type) { void *out=NULL, *tocopy=NULL; uint8_t u8=0; /* Equivalent of minimum in signed with BZERO. */ int16_t s16=INT16_MAX; /* Equivalend of maximum in unsigned with BZERO. */ int32_t s32=INT32_MAX; /* Equivalend of maximum in unsigned with BZERO. */ int64_t s64=INT64_MAX; /* Equivalend of maximum in unsigned with BZERO. */ switch(type) { /* Types with no special treatment: */ case GAL_TYPE_BIT: case GAL_TYPE_UINT8: case GAL_TYPE_INT16: case GAL_TYPE_INT32: case GAL_TYPE_INT64: case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: case GAL_TYPE_STRING: case GAL_TYPE_STRLL: out = gal_blank_alloc_write(type); break; /* Types that need values from their opposite-signed types. */ case GAL_TYPE_INT8: tocopy=&u8; break; case GAL_TYPE_UINT16: tocopy=&s16; break; case GAL_TYPE_UINT32: tocopy=&s32; break; case GAL_TYPE_UINT64: tocopy=&s64; break; default: error(EXIT_FAILURE, 0, "%s: type code %u not recognized as a Gnuastro " "data type", __func__, type); } /* If `gal_blank_alloc_write' wasn't used (copy!=NULL), then allocate the necessary space and fill it in. Note that the width of the signed and unsigned values doesn't differ, so we can use the actual input type. */ if(tocopy) { out = gal_data_malloc_array(type, 1, __func__, "out"); memcpy(out, tocopy, gal_type_sizeof(type)); } /* Return. */ return out; } /* CFITSIO doesn't remove the two single quotes around the string value, so the strings it reads are like: 'value ', or 'some_very_long_value'. To use the value, it is commonly necessary to remove the single quotes (and possible extra spaces). This function will modify the string in its own allocated space. You can use this to later free the original string (if it was allocated). */ void gal_fits_key_clean_str_value(char *string) { int end; /* Has to be int because size_t is always >=0. */ char *c, *cf; /* Start from the second last character (the last is a single quote) and go down until you hit a non-space character. This will also work when there is no space characters between the last character of the value and ending single-quote: it will be set to '\0' after this loop. */ for(end=strlen(string)-2;end>=0;--end) if(string[end]!=' ') break; /* Shift all the characters after the first one (which is a `'' back by one and put the string ending characters on the `end'th element. */ cf=(c=string)+end; do *c=*(c+1); while(++cnext=keysll[i+1]; \\ Put a name and type for each element. gal_fits_key_read_from_ptr(fptr, keysll, 0, 0); \\ use the values as you like. gal_data_array_free(keysll, N, 1); If the `array' pointer of each keyword's dataset is not NULL, then it is assumed that the space has already been allocated. If it is NULL, then space will be allocated internally here. Strings need special consideration: the reason is that generally, `gal_data_t' needs to also allow for array of strings (as it supports arrays of integers for example). Hence two allocations will be done here (one if `array!=NULL') and `keysll[i].array' must be interpretted as `char **': one allocation for the pointer, one for the actual characters. You don't have to worry about the freeing, `gal_data_array_free' will free both allocations. So to read a string, one easy way would be the following: char *str, **strarray; strarr = keysll[i].array; str = strarray[0]; If CFITSIO is unable to read a keyword for any reason the `status' element of the respective `gal_data_t' will be non-zero. You can check the successful reading of the keyword from the `status' value in each keyword's `gal_data_t'. If it is zero, then the keyword was found and succesfully read. Otherwise, it a CFITSIO status value. You can use CFITSIO's error reporting tools or `gal_fits_io_error' for reporting the reason. A tip: when the keyword doesn't exist, then CFITSIO's status value will be `KEY_NO_EXIST'. CFITSIO will start searching for the keywords from the last place in the header that it searched for a keyword. So it is much more efficient if the order that you ask for keywords is based on the order they are stored in the header. */ void gal_fits_key_read_from_ptr(fitsfile *fptr, gal_data_t *keysll, int readcomment, int readunit) { void *valueptr; char **strarray; gal_data_t *tmp; /* Get the desired keywords. */ for(tmp=keysll;tmp!=NULL;tmp=tmp->next) if(tmp->name) { /* Initialize the status: */ tmp->status=0; /* For each keyword, this function stores one value currently. So set the size and ndim to 1. But first allocate dsize if it wasn't already allocated. */ if(tmp->dsize==NULL) tmp->dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, 1, __func__, "tmp->dsize"); tmp->ndim=tmp->size=tmp->dsize[0]=1; /* When the type is a string, `tmp->array' is an array of pointers to a separately allocated piece of memory. So we have to allocate that space here. If its not a string, then the allocated space above is enough to keep the value.*/ switch(tmp->type) { case GAL_TYPE_STRING: errno=0; tmp->array=strarray=( tmp->array ? tmp->array : gal_data_malloc_array(tmp->type, 1, __func__, "tmp->array") ); valueptr=strarray[0]=malloc(FLEN_VALUE * sizeof *strarray[0]); if(strarray[0]==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for strarray[0]", __func__, FLEN_VALUE * sizeof *strarray[0]); break; default: tmp->array=valueptr=( tmp->array ? tmp->array : gal_data_malloc_array(tmp->type, 1, __func__, "tmp->array") ); } /* Allocate space for the keyword comment if necessary.*/ if(readcomment) { errno=0; tmp->comment=calloc(FLEN_COMMENT, sizeof *tmp->comment); if(tmp->comment==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for tmp->comment", __func__, FLEN_COMMENT * sizeof *tmp->comment); } else tmp->comment=NULL; /* Allocate space for the keyword unit if necessary. Note that since there is no precise CFITSIO length for units, we will use the `FLEN_COMMENT' length for units too (theoretically, the unit might take the full remaining area in the keyword). Also note that the unit is only optional, so it needs a separate CFITSIO function call which is done here.*/ if(readunit) { /* Allocate space for the unit and read it in. */ errno=0; tmp->unit=calloc(FLEN_COMMENT, sizeof *tmp->unit); if(tmp->unit==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for tmp->unit", __func__, FLEN_COMMENT * sizeof *tmp->unit); fits_read_key_unit(fptr, tmp->name, tmp->unit, &tmp->status); /* If the string is empty, free the space and set it to NULL. */ if(tmp->unit[0]=='\0') {free(tmp->unit); tmp->unit=NULL;} } else tmp->unit=NULL; /* Read the keyword and place its value in the pointer. */ fits_read_key(fptr, gal_fits_type_to_datatype(tmp->type), tmp->name, valueptr, tmp->comment, &tmp->status); /* If the comment was empty, free the space and set it to zero. */ if(tmp->comment && tmp->comment[0]=='\0') {free(tmp->comment); tmp->comment=NULL;} /* Strings need to be cleaned (CFITSIO puts `'' around them with some (possiblly) extra space on the two ends of the string. */ } } /* Same as `gal_fits_read_keywords_fptr', but accepts the filename and HDU as input instead of an already opened CFITSIO `fitsfile' pointer. */ void gal_fits_key_read(char *filename, char *hdu, gal_data_t *keysll, int readcomment, int readunit) { size_t len; int status=0; char *ffname; fitsfile *fptr; /* Add hdu to filename: */ errno=0; len=strlen(filename)+strlen(hdu)+4; ffname=malloc(len*sizeof *ffname); if(ffname==NULL) error(EXIT_FAILURE, errno, "%s: %zu characters", __func__, len); sprintf(ffname, "%s[%s#]", filename, hdu); /* Open the FITS file: */ if( fits_open_file(&fptr, ffname, READONLY, &status) ) gal_fits_io_error(status, "reading this FITS file"); /* Read the keywords. */ gal_fits_key_read_from_ptr(fptr, keysll, readcomment, readunit); /* Close the FITS file. */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); /* Clean up. */ free(ffname); } /* Add on keyword to the list of header keywords that need to be added to a FITS file. In the end, the keywords will have to be freed, so it is important to know before hand if they were allocated or not. If not, they don't need to be freed. NOTE FOR STRINGS: the value should be the pointer to the string its-self (char *), not a pointer to a pointer (char **). */ void gal_fits_key_list_add(gal_fits_list_key_t **list, uint8_t type, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit) { gal_fits_list_key_t *newnode; /* Allocate space for the new node and fill it in. */ errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating new node", __func__); newnode->type=type; newnode->keyname=keyname; newnode->value=value; newnode->comment=comment; newnode->unit=unit; newnode->kfree=kfree; /* Free pointers after using them. */ newnode->vfree=vfree; newnode->cfree=cfree; newnode->next=*list; *list=newnode; } void gal_fits_key_list_add_end(gal_fits_list_key_t **list, uint8_t type, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit) { gal_fits_list_key_t *newnode, *tmp; /* Allocate space for the new node and fill it in. */ errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocation of new node", __func__); newnode->type=type; newnode->keyname=keyname; newnode->value=value; newnode->comment=comment; newnode->unit=unit; newnode->kfree=kfree; /* Free pointers after using them. */ newnode->vfree=vfree; newnode->cfree=cfree; if(*list) /* List is already full, add this node to the end */ { /* After this line, tmp points to the last node. */ tmp=*list; while(tmp->next!=NULL) tmp=tmp->next; tmp->next=newnode; newnode->next=NULL; } else /* List is empty */ { newnode->next=*list; *list=newnode; } } void gal_fits_key_write_filename(char *keynamebase, char *filename, gal_fits_list_key_t **list) { char *keyname, *value; size_t numkey=1, maxlength; size_t i, j, len=strlen(filename), thislen; /* When you give string arguments, CFITSIO puts them within two ''s, so the actual length available is two less. It seems this length also didn't include the null character, so, ultimately you have to take three from it.*/ maxlength=FLEN_VALUE-3; i=0; while(i0;--j) if(value[j]=='/') { value[j+1]='\0'; break; } if(j==0) error(EXIT_FAILURE, 0, "%s: the filename `%sP has at least one " "span of %zu characters without a `/`. It cannot be " "written to the header of the output fits file", __func__, filename, maxlength); /* Convert the last useful character and save the file name.*/ gal_fits_key_list_add_end(list, GAL_TYPE_STRING, keyname, 1, value, 1, NULL, 0, NULL); i+=j+1; } } } /* Write the WCS header string into a FITS files*/ void gal_fits_key_write_wcsstr(fitsfile *fptr, char *wcsstr, int nkeyrec) { size_t i; int h, status=0; char *cp, *cpf, blankrec[80], titlerec[80]; /* Set the last element of the blank array. */ cpf=blankrec+79; *cpf='\0'; titlerec[79]='\0'; cp=blankrec; do *cp=' '; while(++cpvalue) { if( fits_update_key(fptr, gal_fits_type_to_datatype(tmp->type), tmp->keyname, tmp->value, tmp->comment, &status) ) gal_fits_io_error(status, NULL); } else { if(fits_update_key_null(fptr, tmp->keyname, tmp->comment, &status)) gal_fits_io_error(status, NULL); } /* Write the units if it was given. */ if( tmp->unit && fits_write_key_unit(fptr, tmp->keyname, tmp->unit, &status) ) gal_fits_io_error(status, NULL); /* Free the value pointer if desired: */ if(tmp->kfree) free(tmp->keyname); if(tmp->vfree) free(tmp->value); if(tmp->cfree) free(tmp->comment); /* Keep the pointer to the next keyword and free the allocated space for this keyword.*/ ttmp=tmp->next; free(tmp); tmp=ttmp; } /* Set it to NULL so it isn't mistakenly used later. */ *keylist=NULL; } void gal_fits_key_write_version(fitsfile *fptr, gal_fits_list_key_t *headers, char *program_name) { size_t i; int status=0; char *gitdescribe; char cfitsioversion[20]; char *cp, *cpf, blankrec[80], titlerec[80]; /* Before WCSLIB 5.0, the wcslib_version function was not defined. Sometime in the future were everyone has moved to more recent versions of WCSLIB, we can remove this macro and its check in configure.ac.*/ #if GAL_CONFIG_HAVE_WCSLIB_VERSION == 1 int wcslibvers[3]; char wcslibversion[20]; const char *wcslibversion_const; #endif /* Set the last element of the blank array. */ cpf=blankrec+79; *cpf='\0'; titlerec[79]='\0'; cp=blankrec; do *cp=' '; while(++cpnext) { /* Recall that the order is the opposite (this is a last-in-first-out list. */ if(key->status==0) { switch(i) { case 4: if(unit) {str = key->array; *unit = *str; *str=NULL;} break; case 3: if(name) {str = key->array; *name = *str; *str=NULL;} break; case 2: bscale = *(double *)(key->array); break; case 1: str = key->array; bzero_str = *str; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " "fix the problem. For some reason, there are more " "keywords requested ", __func__, PACKAGE_BUGREPORT); } } ++i; } /* If a type correction is necessary, then do it. */ if( !isnan(bscale) || bzero_str ) fits_type_correct(type, bscale, bzero_str); /* Allocate the array to keep the dimension size and fill it in, note that its order is the opposite of naxes. */ *dsize=gal_data_malloc_array(GAL_TYPE_INT64, *ndim, __func__, "dsize"); for(i=0; i<*ndim; ++i) (*dsize)[i]=naxes[*ndim-1-i]; /* Clean up. Note that bzero_str, gets freed by `gal_data_free' (which is called by `gal_list_data_free'. */ gal_list_data_free(keysll); } /* Read a FITS image HDU into a Gnuastro data structure. */ gal_data_t * gal_fits_img_read(char *filename, char *hdu, size_t minmapsize, size_t hstartwcs, size_t hendwcs) { void *blank; long *fpixel; fitsfile *fptr; gal_data_t *img; size_t i, ndim, *dsize; char *name=NULL, *unit=NULL; int status=0, type, anyblank; /* Check HDU for realistic conditions: */ fptr=gal_fits_hdu_open_format(filename, hdu, 0); /* Get the info and allocate the data structure. */ gal_fits_img_info(fptr, &type, &ndim, &dsize, &name, &unit); /* Check if there is any dimensions (the first header can sometimes have no images). */ if(ndim==0) error(EXIT_FAILURE, 0, "%s (hdu: %s) has 0 dimensions! The most common " "cause for this is a wrongly specified HDU. In some FITS images, " "the first HDU doesn't have any data, the data is in subsequent " "extensions. So probably reading the second HDU (with `--hdu=1' " "or `-h1') will solve the problem (following CFITSIO's " "convention, currently HDU counting starts from 0)." , filename, hdu); /* Set the fpixel array (first pixel in all dimensions). Note that the `long' type will not be larger than 64-bits, so, we'll just assume it is 64-bits for space allocation. On 32-bit systems, this won't be a problem, the space will be written/read as 32-bit `long' any way, we'll just have a few empty bytes that will be freed anyway at the end of this function. */ fpixel=gal_data_malloc_array(GAL_TYPE_INT64, ndim, __func__, "fpixel"); for(i=0;isize, blank, img->array, &anyblank, &status); if(status) gal_fits_io_error(status, NULL); free(fpixel); free(blank); /* Read the WCS structure (if the FITS file has any). */ img->wcs=gal_wcs_read_fitsptr(fptr, hstartwcs, hendwcs, &img->nwcs); /* Close the input FITS file. */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); /* Return the filled data structure */ return img; } /* The user has specified an input file + extension, and your program needs this input to be a special type. For such cases, this function can be used to convert the input file to the desired type. */ gal_data_t * gal_fits_img_read_to_type(char *inputname, char *hdu, uint8_t type, size_t minmapsize, size_t hstartwcs, size_t hendwcs) { gal_data_t *in, *converted; /* Read the specified input image HDU. */ in=gal_fits_img_read(inputname, hdu, minmapsize, hstartwcs, hendwcs); /* If the input had another type, convert it to float. */ if(in->type!=type) { converted=gal_data_copy_to_new_type(in, type); gal_data_free(in); in=converted; } /* Return the final structure. */ return in; } gal_data_t * gal_fits_img_read_kernel(char *filename, char *hdu, size_t minmapsize) { size_t i; int check=0; double sum=0; gal_data_t *kernel; float *f, *fp, tmp; /* Read the image as a float and if it has a WCS structure, free it. */ kernel=gal_fits_img_read_to_type(filename, hdu, GAL_TYPE_FLOAT32, minmapsize, 0, 0); if(kernel->wcs) { wcsfree(kernel->wcs); kernel->wcs=NULL; } /* Check if the size along each dimension of the kernel is an odd number. If they are all an odd number, then the for each dimension, check will be incremented once. */ for(i=0;indim;++i) check += kernel->dsize[i]%2; if(check!=kernel->ndim) error(EXIT_FAILURE, 0, "%s: the kernel image has to have an odd number " "of pixels in all dimensions (there has to be one element/pixel " "in the center). At least one of the dimensions of %s (hdu: %s) " "doesn't have an odd number of pixels", __func__, filename, hdu); /* If there are any NaN pixels, set them to zero and normalize it. A blank pixel in a kernel is going to make a completely blank output.*/ fp=(f=kernel->array)+kernel->size; do { if(isnan(*f)) *f=0.0f; else sum+=*f; } while(++farray; do *f++ *= 1/sum; while(farray; for(i=0;isize/2;++i) { tmp=f[i]; f[i]=f[ kernel->size - i - 1 ]; f[ kernel->size - i - 1 ]=tmp; } /* Return the kernel*/ return kernel; } /* This function will write all the data array information (including its WCS information) into a FITS file, but will not close it. Instead it will pass along the FITS pointer for further modification. */ fitsfile * gal_fits_img_write_to_ptr(gal_data_t *input, char *filename) { void *blank; int64_t *i64; fitsfile *fptr; uint64_t *u64, *u64f; long fpixel=1, *naxes; char *wcsstr, *u64key; size_t i, ndim=input->ndim; int nkeyrec, hasblank, status=0, datatype=0; gal_data_t *i64data, *towrite, *block=gal_tile_block(input); /* If the input is a tile (isn't a contiguous region of memory), then copy it into a contiguous region. */ towrite = input==block ? input : gal_data_copy(input); hasblank=gal_blank_present(towrite, 0); /* Allocate the naxis area. */ naxes=gal_data_malloc_array( ( sizeof(long)==8 ? GAL_TYPE_INT64 : GAL_TYPE_INT32 ), ndim, __func__, "naxes"); /* Open the file for writing */ fptr=gal_fits_open_to_write(filename); /* Fill the `naxes' array (in opposite order, and `long' type): */ for(i=0;idsize[i]; /* Create the FITS file. Unfortunately CFITSIO doesn't have a macro for UINT64, TLONGLONG is only for (signed) INT64. So if the dataset has that type, we'll have to convert it to `INT64' and in the mean-time shift its zero, we will then have to write the BZERO and BSCALE keywords accordingly. */ if(block->type==GAL_TYPE_UINT64) { /* Allocate the necessary space. */ i64data=gal_data_alloc(NULL, GAL_TYPE_INT64, ndim, towrite->dsize, NULL, 0, block->minmapsize, NULL, NULL, NULL); /* Copy the values while making the conversion. */ i64=i64data->array; u64f=(u64=towrite->array)+towrite->size; if(hasblank) { do *i64++ = ( *u64==GAL_BLANK_UINT64 ? GAL_BLANK_INT64 : (*u64 + INT64_MIN) ); while(++u64size, i64data->array, &status); gal_fits_io_error(status, NULL); /* We need to write the BZERO and BSCALE keywords manually. VERY IMPORTANT: this has to be done after writing the array. We cannot write this huge integer as a variable, so we'll simply write the full record/card. It is just important that the string be larger than 80 characters, CFITSIO will trim the rest of the string. */ u64key="BZERO = 9223372036854775808 / Offset of data "; fits_write_record(fptr, u64key, &status); u64key="BSCALE = 1 / Default scaling factor "; fits_write_record(fptr, u64key, &status); gal_fits_io_error(status, NULL); } else { /* Set the datatype */ datatype=gal_fits_type_to_datatype(block->type); /* Create the FITS file. */ fits_create_img(fptr, gal_fits_type_to_bitpix(towrite->type), ndim, naxes, &status); gal_fits_io_error(status, NULL); /* Write the image into the file. */ fits_write_img(fptr, datatype, fpixel, towrite->size, towrite->array, &status); gal_fits_io_error(status, NULL); } /* Remove the two comment lines put by CFITSIO. Note that in some cases, it might not exist. When this happens, the status value will be non-zero. We don't care about this error, so to be safe, we will just reset the status variable after these calls. */ fits_delete_key(fptr, "COMMENT", &status); fits_delete_key(fptr, "COMMENT", &status); status=0; /* If we have blank pixels, we need to define a BLANK keyword when we are dealing with integer types. */ if(hasblank) switch(towrite->type) { case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: /* Do nothing! Since there are much fewer floating point types (that don't need any BLANK keyword), we are checking them.*/ break; default: blank=gal_fits_key_img_blank(towrite->type); if(fits_write_key(fptr, datatype, "BLANK", blank, "Pixels with no data.", &status) ) gal_fits_io_error(status, "adding the BLANK keyword"); free(blank); } /* Write the extension name to the header. */ if(towrite->name) fits_write_key(fptr, TSTRING, "EXTNAME", towrite->name, "", &status); /* Write the units to the header. */ if(towrite->unit) fits_write_key(fptr, TSTRING, "BUNIT", towrite->unit, "", &status); /* Write comments if they exist. */ if(towrite->comment) fits_write_comment(fptr, towrite->comment, &status); /* If a WCS structure is present, write it in */ if(towrite->wcs) { /* Decompose the `PCi_j' matrix and `CDELTi' vector. */ gal_wcs_decompose_pc_cdelt(towrite->wcs); /* Convert the WCS information to text. */ status=wcshdo(WCSHDO_safe, towrite->wcs, &nkeyrec, &wcsstr); if(status) error(EXIT_FAILURE, 0, "%s: wcshdo ERROR %d: %s", __func__, status, wcs_errmsg[status]); gal_fits_key_write_wcsstr(fptr, wcsstr, nkeyrec); } /* Report any errors if we had any */ free(naxes); gal_fits_io_error(status, NULL); if(towrite!=input) gal_data_free(towrite); return fptr; } void gal_fits_img_write(gal_data_t *data, char *filename, gal_fits_list_key_t *headers, char *program_string) { int status=0; fitsfile *fptr; /* Write the data array into a FITS file and keep it open: */ fptr=gal_fits_img_write_to_ptr(data, filename); /* Write all the headers and the version information. */ gal_fits_key_write_version(fptr, headers, program_string); /* Close the FITS file. */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); } void gal_fits_img_write_to_type(gal_data_t *data, char *filename, gal_fits_list_key_t *headers, char *program_string, int type) { /* If the input dataset is not the correct type, then convert it, otherwise, use the input data structure. */ gal_data_t *towrite = (data->type==type ? data : gal_data_copy_to_new_type(data, type)); /* Write the converted dataset into an image. */ gal_fits_img_write(towrite, filename, headers, program_string); /* Free the dataset if it was allocated. */ if(towrite!=data) gal_data_free(towrite); } /* This function is mainly useful when you want to make FITS files in parallel (from one main WCS structure, with just differing CRPIX) for two reasons: - When a large number of FITS images (with WCS) need to be created in parallel, it can be much more efficient to write the header's WCS keywords once at first, write them in the FITS file, then just correct the CRPIX values. - WCSLIB's header writing function is not thread safe. So when writing FITS images in parallel, we can't write the header keywords in each thread. */ void gal_fits_img_write_corr_wcs_str(gal_data_t *input, char *filename, char *wcsstr, int nkeyrec, double *crpix, gal_fits_list_key_t *headers, char *program_string) { int status=0; fitsfile *fptr; /* The data should not have any WCS structure for this function. */ if(input->wcs) error(EXIT_FAILURE, 0, "%s: input must not have WCS meta-data", __func__); /* Write the data array into a FITS file and keep it open. */ fptr=gal_fits_img_write_to_ptr(input, filename); /* Write the WCS headers into the FITS file. */ gal_fits_key_write_wcsstr(fptr, wcsstr, nkeyrec); /* Update the CRPIX keywords. Note that we don't want to change the values in the WCS information of gal_data_t. Because, it often happens that things are done in parallel, so we don't want to touch the original version, we just want to change the copied version. */ if(crpix) { fits_update_key(fptr, TDOUBLE, "CRPIX1", &crpix[0], NULL, &status); fits_update_key(fptr, TDOUBLE, "CRPIX2", &crpix[1], NULL, &status); if(input->ndim==3) fits_update_key(fptr, TDOUBLE, "CRPIX3", &crpix[2], NULL, &status); gal_fits_io_error(status, NULL); } /* Write all the headers and the version information. */ gal_fits_key_write_version(fptr, headers, program_string); /* Close the file and return. */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); } /**************************************************************/ /********** Table ************/ /**************************************************************/ /* Get the size of a table HDU. CFITSIO doesn't use size_t, also we want to check status here.*/ void gal_fits_tab_size(fitsfile *fitsptr, size_t *nrows, size_t *ncols) { long lnrows; int incols, status=0; /* Read the sizes and put them in. */ fits_get_num_rows(fitsptr, &lnrows, &status); fits_get_num_cols(fitsptr, &incols, &status); *ncols=incols; *nrows=lnrows; /* Report an error if any was issued. */ gal_fits_io_error(status, NULL); } int gal_fits_tab_format(fitsfile *fitsptr) { int status=0; char value[FLEN_VALUE]; fits_read_key(fitsptr, TSTRING, "XTENSION", value, NULL, &status); if(status==0) { if(!strcmp(value, "TABLE")) return GAL_TABLE_FORMAT_AFITS; else if(!strcmp(value, "BINTABLE")) return GAL_TABLE_FORMAT_BFITS; else error(EXIT_FAILURE, 0, "%s: the `XTENSION' keyword of this FITS " "table (`%s') doesn't have a standard value", __func__, value); } else { if(status==KEY_NO_EXIST) error(EXIT_FAILURE, 0, "%s: input fitsfile pointer isn't a table", __func__); else gal_fits_io_error(status, NULL); } error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can fix it. " "Control should not have reached the end of this function", __func__, PACKAGE_BUGREPORT); return -1; } /* The general format of the TDISPn keywords in FITS is like this: `Tw.p', where `T' specifies the general format, `w' is the width to be given to this column and `p' is the precision. For integer types, percision is actually the minimum number of integers, for floats, it is the number of decimal digits beyond the decimal point. */ static void set_display_format(char *tdisp, gal_data_t *data, char *filename, char *hdu, char *keyname) { int isanint=0; char *tailptr; /* First, set the general display format */ switch(tdisp[0]) { case 'A': data->disp_fmt=GAL_TABLE_DISPLAY_FMT_STRING; break; case 'I': isanint=1; data->disp_fmt=GAL_TABLE_DISPLAY_FMT_DECIMAL; break; case 'O': isanint=1; data->disp_fmt=GAL_TABLE_DISPLAY_FMT_OCTAL; break; case 'Z': isanint=1; data->disp_fmt=GAL_TABLE_DISPLAY_FMT_HEX; break; case 'F': data->disp_fmt=GAL_TABLE_DISPLAY_FMT_FLOAT; break; case 'E': case 'D': data->disp_fmt=GAL_TABLE_DISPLAY_FMT_EXP; break; case 'G': data->disp_fmt=GAL_TABLE_DISPLAY_FMT_GENERAL; break; default: error(EXIT_FAILURE, 0, "%s (hdu: %s): Format character `%c' in the " "value (%s) of the keyword %s not recognized in %s", filename, hdu, tdisp[0], tdisp, keyname, __func__); } /* Parse the rest of the string to see if a width and precision are given or not. */ data->disp_width=strtol(&tdisp[1], &tailptr, 0); switch(*tailptr) { case '.': /* Width is set, go onto finding the precision. */ data->disp_precision = strtol(&tailptr[1], &tailptr, 0); if(*tailptr!='\0') error(EXIT_FAILURE, 0, "%s (hdu: %s): The value `%s' of the " "`%s' keyword could not recognized (it doesn't finish after " "the precision) in %s", filename, hdu, tdisp, keyname, __func__); break; case '\0': /* No precision given, use a default value. */ data->disp_precision = ( isanint ? GAL_TABLE_DEF_PRECISION_INT : GAL_TABLE_DEF_PRECISION_FLT ); break; default: error(EXIT_FAILURE, 0, "%s (hdu: %s): The value `%s' of the " "`%s' keyword could not recognized (it doesn't have a `.', or " "finish, after the width) in %s", filename, hdu, tdisp, keyname, __func__); } } /* The FITS standard for binary tables (not ASCII tables) does not allow unsigned types for short, int and long types, or signed char! So it has `TSCALn' and `TZEROn' to scale the signed types to an unsigned type. It does this internally, but since we need to define our data type and allocate space for it before actually reading the array, it is necessary to do this setting here. */ static void fits_correct_bin_table_int_types(gal_data_t *allcols, int tfields, int *tscal, long long *tzero) { size_t i; for(i=0;inext) { /* Allocate the necessary data structure (including the array) for this column. */ dsize=numrows; gal_list_data_add_alloc(&out, NULL, allcols[ind->v].type, 1, &dsize, NULL, 0, minmapsize, allcols[ind->v].name, allcols[ind->v].unit, allcols[ind->v].comment); /* For a string column, we need an allocated array for each element, even in binary values. This value should be stored in the disp_width element of the data structure, which is done automatically in `gal_fits_table_info'. */ if(out->type==GAL_TYPE_STRING) for(i=0;iarray; errno=0; strarr[i]=calloc(allcols[ind->v].disp_width+1, sizeof *strarr[i]); if(strarr[i]==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for " "strarr[%zu]", __func__, (allcols[ind->v].disp_width+1) * sizeof *strarr[i], i); } /* Allocate a blank value for the given type and read/store the column using CFITSIO. Afterwards, free the blank value. */ blank=gal_blank_alloc_write(out->type); fits_read_col(fptr, gal_fits_type_to_datatype(out->type), ind->v+1, 1, 1, out->size, blank, out->array, &anynul, &status); gal_fits_io_error(status, NULL); free(blank); } /* Close the FITS file */ fits_close_file(fptr, &status); gal_fits_io_error(status, NULL); return out; } /* This function will allocate new copies for all elements to have the same length as the maximum length and set all trailing elements to `\0' for those that are shorter than the length. The return value is the allocated space. If the dataset is not a string, the returned value will be -1 (largest number of `size_t'). */ static size_t fits_string_fixed_alloc_size(gal_data_t *data) { size_t i, j, maxlen=0; char *tmp, **strarr=data->array; /* Return 0 if the dataset is not a string. */ if(data->type!=GAL_TYPE_STRING) return -1; /* Get the maximum length. */ for(i=0;isize;++i) maxlen = strlen(strarr[i])>maxlen ? strlen(strarr[i]) : maxlen; /* For all elements, check the length and if they aren't equal to maxlen, then allocate a maxlen sized array and put the values in. */ for(i=0;isize;++i) { /* Allocate (and clear) the space for the new string. We want it to be cleared, so when the strings are smaller, the rest of the space is filled with '\0' (ASCII for 0) values.*/ errno=0; tmp=calloc(maxlen+1, sizeof *strarr[i]); if(tmp==NULL) error(EXIT_FAILURE, 0, "%s: %zu bytes for tmp", __func__, (maxlen+1)*sizeof *strarr[i]); /* Put the old array into the newly allocated space. `tmp' was cleared (all values set to `\0', so we don't need to set the final one explicity after the copy.*/ for(j=0;strarr[i][j]!='\0';++j) tmp[j]=strarr[i][j]; /* Free the old array and put in the new one. */ free(strarr[i]); strarr[i]=tmp; } /* Return the allocated space. */ return maxlen+1; } static void fits_table_prepare_arrays(gal_data_t *cols, size_t numcols, int tableformat, char ***outtform, char ***outttype, char ***outtunit) { size_t i=0; gal_data_t *col; char fmt[2], lng[3]; char *blank, **tform, **ttype, **tunit; /* Allocate the arrays to keep the `tform' values */ errno=0; tform=*outtform=malloc(numcols*sizeof *tform); if(tform==NULL) error(EXIT_FAILURE, 0, "%s: %zu bytes for tform", __func__, numcols*sizeof *tform); errno=0; ttype=*outttype=malloc(numcols*sizeof *ttype); if(ttype==NULL) error(EXIT_FAILURE, 0, "%s: %zu bytes for ttype", __func__, numcols*sizeof *ttype); errno=0; tunit=*outtunit=malloc(numcols*sizeof *tunit); if(tunit==NULL) error(EXIT_FAILURE, 0, "%s: %zu bytes for tunit", __func__, numcols*sizeof *tunit); /* Go over each column and fill in these arrays. */ for(col=cols; col!=NULL; col=col->next) { /* Set the `ttype' and `tunit' values: */ asprintf(&ttype[i], "%s", col->name ? col->name : ""); asprintf(&tunit[i], "%s", col->unit ? col->unit : ""); /* FITS's TFORM depends on the type of FITS table, so work differently. */ switch(tableformat) { /* FITS ASCII table. */ case GAL_TABLE_FORMAT_AFITS: /* Fill the printing format. */ gal_tableintern_col_print_info(col, GAL_TABLE_FORMAT_AFITS, fmt, lng); /* We need to check if the blank value needs is larger than the expected width or not. Its initial width is set the output of the function above, but if the value is larger, `asprintf' (which is used) will make it wider. */ blank = ( gal_blank_present(col, 0) ? gal_blank_as_string(col->type, col->disp_width) : NULL ); /* Adjust the width. */ if(blank) { col->disp_width = ( strlen(blank) > col->disp_width ? strlen(blank) : col->disp_width ); free(blank); } /* Print the value to be used as TFORMn: */ switch(col->type) { case GAL_TYPE_STRING: case GAL_TYPE_UINT8: case GAL_TYPE_INT8: case GAL_TYPE_UINT16: case GAL_TYPE_INT16: case GAL_TYPE_UINT32: case GAL_TYPE_INT32: case GAL_TYPE_UINT64: case GAL_TYPE_INT64: asprintf(&tform[i], "%c%d", fmt[0], col->disp_width); break; case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: asprintf(&tform[i], "%c%d.%d", fmt[0], col->disp_width, col->disp_precision); break; default: error(EXIT_FAILURE, 0, "%s: col->type code %d not recognized", __func__, col->type); } break; /* FITS binary table. */ case GAL_TABLE_FORMAT_BFITS: /* If this is a string column, set all the strings to same size, then write the value of tform depending on the type. */ col->disp_width=fits_string_fixed_alloc_size(col); fmt[0]=gal_fits_type_to_bin_tform(col->type); if( col->type==GAL_TYPE_STRING ) asprintf(&tform[i], "%d%c", col->disp_width, fmt[0]); else asprintf(&tform[i], "%c", fmt[0]); break; default: error(EXIT_FAILURE, 0, "%s: tableformat code %d not recognized", __func__, tableformat); } /* Increment the column index. */ ++i; } } /* Write the TNULLn keywords into the FITS file. Note that this depends on the type of the table: for an ASCII table, all the columns need it. For a binary table, only the non-floating point ones (even if they don't have NULL values) must have it. */ static void fits_write_tnull_tcomm(fitsfile *fptr, gal_data_t *col, int tableformat, size_t colnum, char *tform) { void *blank; int status=0; char *c, *keyname, *bcomment; /* Write the NULL value */ switch(tableformat) { case GAL_TABLE_FORMAT_AFITS: /* Print the keyword and value. */ asprintf(&keyname, "TNULL%zu", colnum); blank=gal_blank_as_string(col->type, col->disp_width); /* When in exponential form (`tform' starting with `E'), CFITSIO writes a NaN value as `NAN', but when in floating point form (`tform' starting with `F'), it writes it as `nan'. So in the former case, we need to convert the string to upper case. */ if(tform[0]=='E' || tform[0]=='e') for(c=blank; *c!='\0'; ++c) *c=toupper(*c); /* Write in the header. */ fits_write_key(fptr, TSTRING, keyname, blank, "blank value for this column", &status); /* Clean up. */ free(keyname); free(blank); break; case GAL_TABLE_FORMAT_BFITS: /* FITS binary tables don't accept NULL values for floating point or string columns. For floating point is must be NaN and for strings it is a blank string. */ if( col->type!=GAL_TYPE_FLOAT32 && col->type!=GAL_TYPE_FLOAT64 && col->type!=GAL_TYPE_STRING ) { blank=gal_blank_alloc_write(col->type); asprintf(&keyname, "TNULL%zu", colnum); fits_write_key(fptr, gal_fits_type_to_datatype(col->type), keyname, blank, "blank value for this column", &status); gal_fits_io_error(status, NULL); free(keyname); free(blank); } break; default: error(EXIT_FAILURE, 0, "%s: tableformat code %d not recognized", __func__, tableformat); } /* Write the comments if there is any. */ if(col->comment) { asprintf(&keyname, "TCOMM%zu", colnum); asprintf(&bcomment, "comment for field %zu", colnum); fits_write_key(fptr, TSTRING, keyname, col->comment, bcomment, &status); gal_fits_io_error(status, NULL); free(keyname); free(bcomment); } } /* Write the given columns (a linked list of `gal_data_t') into a FITS table.*/ void gal_fits_tab_write(gal_data_t *cols, gal_list_str_t *comments, int tableformat, char *filename, char *extname) { void *blank; fitsfile *fptr; gal_data_t *col; size_t i, numrows=-1; gal_list_str_t *strt; char **ttype, **tform, **tunit; int tbltype, numcols=0, status=0; /* Make sure all the input columns have the same number of elements */ for(col=cols; col!=NULL; col=col->next) { if(numrows==-1) numrows=col->size; else if(col->size!=numrows) error(EXIT_FAILURE, 0, "%s: the number of records/rows in the input " "columns are not equal", __func__); ++numcols; } /* Open the FITS file for writing. */ fptr=gal_fits_open_to_write(filename); /* prepare necessary arrays and if integer type columns have blank values, write the TNULLn keywords into the FITS file. */ fits_table_prepare_arrays(cols, numcols, tableformat, &tform, &ttype, &tunit); /* Make the FITS file pointer. Note that tableformat was checked in `fits_table_prepare_arrays'. */ tbltype = tableformat==GAL_TABLE_FORMAT_AFITS ? ASCII_TBL : BINARY_TBL; fits_create_tbl(fptr, tbltype, numrows, numcols, ttype, tform, tunit, extname, &status); gal_fits_io_error(status, NULL); /* Write the columns into the file and also write the blank values into the header when necessary. */ i=0; for(col=cols; col!=NULL; col=col->next) { /* Write the blank value into the header and return a pointer to it. Otherwise, */ fits_write_tnull_tcomm(fptr, col, tableformat, i+1, tform[i]); /* Set the blank pointer if its necessary, note that strings don't need a blank pointer in a FITS ASCII table.*/ blank = ( gal_blank_present(col, 0) ? gal_blank_alloc_write(col->type) : NULL ); if(tableformat==GAL_TABLE_FORMAT_AFITS && col->type==GAL_TYPE_STRING) { if(blank) free(blank); blank=NULL; } /* Write the full column into the table. */ fits_write_colnull(fptr, gal_fits_type_to_datatype(col->type), i+1, 1, 1, col->size, col->array, blank, &status); gal_fits_io_error(status, NULL); /* Clean up and Increment the column counter. */ if(blank) free(blank); ++i; } /* Write the comments if there were any. */ for(strt=comments; strt!=NULL; strt=strt->next) fits_write_comment(fptr, strt->v, &status); /* Write all the headers and the version information. */ gal_fits_key_write_version(fptr, NULL, NULL); /* Clean up and close the FITS file. Note that each element in the `ttype' and `tunit' arrays just points to the respective string in the column data structure, the space for each element of the array wasn't allocated.*/ for(i=0;i Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /*********************************************************************/ /************* Size and allocation *******************/ /*********************************************************************/ int gal_data_dsize_is_different(gal_data_t *first, gal_data_t *second) { size_t i; /* First make sure that the dimensionality is the same. */ if(first->ndim!=second->ndim) return 1; /* Check if the sizes along all dimensions are the same: */ for(i=0;indim;++i) if( first->dsize[i] != second->dsize[i] ) return 1; /* If it got to here, we know the dimensions have the same length. */ return 0; } /* Increment a give pointer depending on the given type. When working with the `array' elements of `gal_data_t', we are actually dealing with `void *' pointers. Pointer arithmetic doesn't apply to `void *', because the system doesn't know how much space each element has to increment the pointer respectively. So, here, we will use the type information to find the increment. This is mainly useful when dealing with the `block' pointer of a tile over a larger image. This function reads the address as a `char *' type (note that `char' is guaranteed to have a size of 1 (byte)). It then increments the `char *' by `increment*sizeof(type)' */ void * gal_data_ptr_increment(void *pointer, size_t increment, uint8_t type) { char *p=(char *)pointer; return p + increment * gal_type_sizeof(type); } /* Find the distance between two void pointers with a given type. See the explanations before `gal_data_ptr_increment'. */ size_t gal_data_ptr_dist(void *earlier, void *later, uint8_t type) { char *e=(char *)earlier, *l=(char *)later; return (l-e)/gal_type_sizeof(type); } /* Allocate an array based on the value of type. Note that the argument `size' is the number of elements, necessary in the array, the number of bytes each element needs will be determined internaly by this function using the datatype argument, so you don't have to worry about it. */ void * gal_data_malloc_array(uint8_t type, size_t size, const char *funcname, const char *varname) { void *array; errno=0; array=malloc( size * gal_type_sizeof(type) ); if(array==NULL) { if(varname) error(EXIT_FAILURE, errno, "%s: %zu bytes couldn't be allocated " "for variable `%s'", funcname ? funcname : __func__, size * gal_type_sizeof(type), varname); else error(EXIT_FAILURE, errno, "%s: %zu bytes couldn't be allocated", funcname ? funcname : __func__, size * gal_type_sizeof(type)); } return array; } void * gal_data_calloc_array(uint8_t type, size_t size, const char *funcname, const char *varname) { void *array; errno=0; array=calloc( size, gal_type_sizeof(type) ); if(array==NULL) { if(varname) error(EXIT_FAILURE, errno, "%s: %zu bytes couldn't be allocated " "for variable `%s'", funcname ? funcname : __func__, size * gal_type_sizeof(type), varname); else error(EXIT_FAILURE, errno, "%s: %zu bytes couldn't be allocated", funcname ? funcname : __func__, size * gal_type_sizeof(type)); } return array; } static void gal_data_mmap(gal_data_t *data, int clear, size_t minmapsize) { int filedes; uint8_t uc=0; char *filename; size_t bsize=data->size*gal_type_sizeof(data->type); /* Check if the .gnuastro folder exists, write the file there. If it doesn't exist, then make the .gnuastro directory.*/ gal_checkset_mkdir(".gnuastro"); /* Set the filename */ gal_checkset_allocate_copy("./.gnuastro/mmap_XXXXXX", &filename); /* Create a zero-sized file and keep its descriptor. */ errno=0; /*filedes=open(filename, O_RDWR | O_CREAT | O_EXCL | O_TRUNC );*/ filedes=mkstemp(filename); if(filedes==-1) error(EXIT_FAILURE, errno, "%s: %s couldn't be created", __func__, filename); /* Make enough space to keep the array data. */ errno=0; if( lseek(filedes, bsize, SEEK_SET) == -1 ) error(EXIT_FAILURE, errno, "%s: %s: unable to change file position by " "%zu bytes", __func__, filename, bsize); /* Write to the newly set file position so the space is allocated. To do this, we are simply writing `uc' (a byte with value 0) into the space we identified by `lseek' (above). This will ensure that this space is set a side for this array and prepare us to use `mmap'. */ if( write(filedes, &uc, 1) == -1) error(EXIT_FAILURE, errno, "%s: %s: unable to write one byte at the " "%zu-th position", __func__, filename, bsize); /* Map the memory. */ errno=0; data->array=mmap(NULL, bsize, PROT_READ | PROT_WRITE, MAP_SHARED, filedes, 0); if(data->array==MAP_FAILED) { if(minmapsize<10000u) fprintf(stderr, "\nIf the processing involves many small mappings " "(along with larger ones), the following error may be " "corrected with a larger value to `minmapsize' (minimum " "number of bytes to use mapping instead of RAM for each " "patch of memory), for example 10000. In this way, mapping " "will only be reserved for larger sizes. The current value is " "%zu.\n\n", minmapsize); error(EXIT_FAILURE, errno, "couldn't map %zu bytes into the file `%s'", bsize, filename); } /* Close the file. */ if( close(filedes) == -1 ) error(EXIT_FAILURE, errno, "%s: %s couldn't be closed", __func__, filename); /* Keep the filename. */ data->mmapname=filename; /* If it was supposed to be cleared, then clear the memory. */ if(clear) memset(data->array, 0, bsize); } /* Initialize the data structure. Some notes: - The `status' value is the only element that cannot be set by this function, it is initialized to zero. - If no `array' is given, a blank array of the given size will be allocated. If it is given the array pointer will be directly put here, so do not free it independently any more. If you want a separate copy of a dataset, you should use `gal_data_copy', not this function. - Space for the `name', `unit', and `comment' strings within the data structure are allocated here. So you can safely use literal strings, or statically allocated ones, or simply the strings from other data structures (and not have to worry about which one to free later). */ void gal_data_initialize(gal_data_t *data, void *array, uint8_t type, size_t ndim, size_t *dsize, struct wcsprm *wcs, int clear, size_t minmapsize, char *name, char *unit, char *comment) { size_t i; size_t data_size_limit = (size_t)(-1); /* Do the simple copying cases. For the display elements, set them all to impossible (negative) values so if not explicitly set by later steps, the default values are used if/when printing.*/ data->flag = 0; data->status = 0; data->next = NULL; data->ndim = ndim; data->type = type; data->block = NULL; data->mmapname = NULL; data->minmapsize = minmapsize; gal_checkset_allocate_copy(name, &data->name); gal_checkset_allocate_copy(unit, &data->unit); gal_checkset_allocate_copy(comment, &data->comment); data->disp_fmt=data->disp_width=data->disp_precision=-1; /* Copy the WCS structure. */ data->wcs=gal_wcs_copy(wcs); /* Allocate space for the dsize array, only if the data are to have any dimensions. Note that in our convention, a number has a `ndim=1' and `dsize[0]=1', A 1D array also has `ndim=1', but `dsize[0]>1'. */ if(ndim) { /* Allocate dsize. */ errno=0; data->dsize=malloc(ndim*sizeof *data->dsize); if(data->dsize==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for data->dsize", __func__, ndim*sizeof *data->dsize); /* Fill in the `dsize' array and in the meantime set `size': */ data->size=1; for(i=0;i= data_size_limit / data->size) error(EXIT_FAILURE, 0, "%s: dimension %zu size is too " "large %zu. Total is out of bounds", __func__, i, dsize[i]); /* Print a warning if the size in this dimension is too large. May happen when the user (mistakenly) writes a negative value in this dimension.. */ if (dsize[i] >= data_size_limit / 2) fprintf(stderr, "%s: WARNING: dsize[%zu] value %zu is probably " "a mistake: it exceeds the limit %zu", __func__, i, dsize[i], data_size_limit / 2); /* Write this dimension's size, also correct the total number of elements. */ data->size *= ( data->dsize[i] = dsize[i] ); } /* Set the array pointer. If an non-NULL array pointer was given, then use it. */ if(array) data->array=array; else { if(data->size) { if( gal_type_sizeof(type)*data->size > minmapsize ) /* Allocate the space into disk (HDD/SSD). */ gal_data_mmap(data, clear, minmapsize); else /* Allocate the space in RAM. */ data->array = ( clear ? gal_data_calloc_array(data->type, data->size, __func__, "data->array") : gal_data_malloc_array(data->type, data->size, __func__, "data->array") ); } else data->array=NULL; /* The given size was zero! */ } } else { data->size=0; data->array=NULL; data->dsize=NULL; } } /* Allocate a data structure based on the given parameters. If you want to force the array into the hdd/ssd (mmap it), then set minmapsize=-1 (largest possible size_t value), in this way, no file will be larger. */ gal_data_t * gal_data_alloc(void *array, uint8_t type, size_t ndim, size_t *dsize, struct wcsprm *wcs, int clear, size_t minmapsize, char *name, char *unit, char *comment) { gal_data_t *out; /* Allocate the space for the actual structure. */ errno=0; out=malloc(sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for gal_data_t", __func__, sizeof *out); /* Initialize the allocated array. */ gal_data_initialize(out, array, type, ndim, dsize, wcs, clear, minmapsize, name, unit, comment); /* Return the final structure. */ return out; } /* Free the allocated contents of a data structure, not the structure itsself. The reason that this function is separate from `gal_data_free' is that the data structure might be allocated as an array (statically like `gal_data_t da[20]', or dynamically like `gal_data_t *da; da=malloc(20*sizeof *da);'). In both cases, a loop will be necessary to delete the allocated contents of each element of the data structure array, but not the structure its self. After that loop, if the array of data structures was statically allocated, you don't have to do anything. If it was dynamically allocated, we just have to run `free(da)'. Since we aren't freeing the `gal_data_t' its-self, after the allocated space for each pointer is freed, the pointer is set to NULL for safety (to avoid possible re-calls). */ void gal_data_free_contents(gal_data_t *data) { size_t i; char **strarr; if(data==NULL) error(EXIT_FAILURE, 0, "%s: the input data structure to " "`gal_data_free_contents' was a NULL pointer", __func__); /* Free all the possible allocations. */ if(data->name) { free(data->name); data->name = NULL; } if(data->unit) { free(data->unit); data->unit = NULL; } if(data->dsize) { free(data->dsize); data->dsize = NULL; } if(data->wcs) { wcsfree(data->wcs); data->wcs = NULL; } if(data->comment) { free(data->comment); data->comment = NULL; } /* If the data type is string, then each element in the array is actually a pointer to the array of characters, so free them before freeing the actual array. */ if(data->type==GAL_TYPE_STRING && data->array) { strarr=data->array; for(i=0;isize;++i) free(strarr[i]); } /* Free the array. */ if(data->mmapname) { /* Delete the file keeping the array. */ remove(data->mmapname); /* Free the file name space. */ free(data->mmapname); /* Set the name pointer to NULL since it has been freed. */ data->mmapname=NULL; } else if(data->array && data->block==NULL) free(data->array); data->array=NULL; } /* Free the contents of the data structure and the data structure itsself. */ void gal_data_free(gal_data_t *data) { if(data) { gal_data_free_contents(data); free(data); } } /*********************************************************************/ /************* Array of data structures ******************/ /*********************************************************************/ /* Allocate an array of data structures and initialize all the values. */ gal_data_t * gal_data_array_calloc(size_t size) { size_t i; gal_data_t *out; /* Allocate the array to keep the structures. */ errno=0; out=malloc(size*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for `out'", __func__, size*sizeof *out); /* Set the pointers to NULL if they didn't exist and the non-pointers to impossible integers (so the caller knows the array is only allocated. `minmapsize' should be set when allocating the array and should be set when you run `gal_data_initialize'. */ for(i=0;iarray, **outstrarr=to->array; /* Sanity check. */ if(from->type!=GAL_TYPE_STRING) error(EXIT_FAILURE, 0, "%s: `from' must have a string type.", __func__); if(from->block) error(EXIT_FAILURE, 0, "%s: tiles not currently supported (`block' " "element must be NULL). Please contact us at %s so we can " "implement this feature", __func__, PACKAGE_BUGREPORT); /* Do the copying. */ for(i=0;isize;++i) { /* Set the pointer. */ switch(to->type) { case GAL_TYPE_UINT8: ptr = (uint8_t *)(to->array) + i; break; case GAL_TYPE_INT8: ptr = (int8_t *)(to->array) + i; break; case GAL_TYPE_UINT16: ptr = (uint16_t *)(to->array) + i; break; case GAL_TYPE_INT16: ptr = (int16_t *)(to->array) + i; break; case GAL_TYPE_UINT32: ptr = (uint32_t *)(to->array) + i; break; case GAL_TYPE_INT32: ptr = (int32_t *)(to->array) + i; break; case GAL_TYPE_UINT64: ptr = (uint64_t *)(to->array) + i; break; case GAL_TYPE_INT64: ptr = (int64_t *)(to->array) + i; break; case GAL_TYPE_FLOAT32: ptr = (float *)(to->array) + i; break; case GAL_TYPE_FLOAT64: ptr = (double *)(to->array) + i; break; case GAL_TYPE_BIT: case GAL_TYPE_STRLL: case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: error(EXIT_FAILURE, 0, "%s: copying to %s type not currently " "supported", __func__, gal_type_name(to->type, 1)); break; default: error(EXIT_FAILURE, 0, "%s: type %d not recognized for to->type", __func__, to->type); } /* Read/put the input into the output. */ if(to->type==GAL_TYPE_STRING) gal_checkset_allocate_copy(strarr[i], &outstrarr[i]); else { if( gal_type_from_string(&ptr, strarr[i], to->type) ) data_copy_to_string_not_parsed(strarr[i], ptr, to->type); } } } /* Macros for copying to a string. */ #define COPY_TO_STR_INT(CTYPE, BLANK, FMT) { \ CTYPE *a=from->array; \ for(i=0;isize;++i) \ { \ if(a[i]!=BLANK) asprintf(&strarr[i], FMT, a[i]); \ else \ gal_checkset_allocate_copy(GAL_BLANK_STRING, &strarr[i]); \ } \ } #define COPY_TO_STR_FLT(CTYPE, BLANK) { \ CTYPE *a=from->array; \ for(i=0;isize;++i) \ { \ if(isnan(BLANK)) isblank = isnan(a[i]) ? 1 : 0; \ else isblank = a[i]==BLANK ? 1 : 0; \ if(isblank==0) asprintf(&strarr[i], "%f", a[i]); \ else gal_checkset_allocate_copy(GAL_BLANK_STRING, &strarr[i]); \ } \ } /* Convert any given type into a string by printing it into the elements of the already allocated `to->array'. */ static void data_copy_to_string(gal_data_t *from, gal_data_t *to) { size_t i; int isblank; char **strarr=to->array, **instrarr=from->array; /* Sanity check */ if(to->type!=GAL_TYPE_STRING) error(EXIT_FAILURE, 0, "%s: `to' must have a string type", __func__); if(from->block) error(EXIT_FAILURE, 0, "%s: tile inputs not currently supported " "(`block' element must be NULL). Please contact us at %s so we " "can implement this feature", __func__, PACKAGE_BUGREPORT); /* Do the copying */ switch(from->type) { case GAL_TYPE_UINT8: COPY_TO_STR_INT(uint8_t, GAL_BLANK_UINT8, "%"PRIu8); break; case GAL_TYPE_INT8: COPY_TO_STR_INT(int8_t, GAL_BLANK_INT8, "%"PRId8); break; case GAL_TYPE_UINT16: COPY_TO_STR_INT(uint16_t, GAL_BLANK_UINT16, "%"PRIu16); break; case GAL_TYPE_INT16: COPY_TO_STR_INT(int16_t, GAL_BLANK_INT16, "%"PRId16); break; case GAL_TYPE_UINT32: COPY_TO_STR_INT(uint32_t, GAL_BLANK_UINT32, "%"PRIu32); break; case GAL_TYPE_INT32: COPY_TO_STR_INT(int32_t, GAL_BLANK_INT32, "%"PRId32); break; case GAL_TYPE_UINT64: COPY_TO_STR_INT(uint64_t, GAL_BLANK_UINT64, "%"PRIu64); break; case GAL_TYPE_INT64: COPY_TO_STR_INT(int64_t, GAL_BLANK_INT64, "%"PRId64); break; case GAL_TYPE_FLOAT32: COPY_TO_STR_FLT(float, GAL_BLANK_FLOAT32); break; case GAL_TYPE_FLOAT64: COPY_TO_STR_FLT(double, GAL_BLANK_FLOAT32); break; case GAL_TYPE_STRING: for(i=0;isize;++i) gal_checkset_allocate_copy(instrarr[i], &strarr[i]); break; case GAL_TYPE_BIT: case GAL_TYPE_STRLL: case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: error(EXIT_FAILURE, 0, "%s: copying to %s type not currently supported", __func__, gal_type_name(from->type, 1)); break; default: error(EXIT_FAILURE, 0, "%s: type %d not recognized for `from->type'", __func__, from->type); } } #define COPY_OT_IT_SET(OT, IT) { \ OT ob, *restrict o=out->array; \ size_t increment=0, num_increment=1; \ size_t mclen=0, contig_len=in->dsize[in->ndim-1]; \ IT ib, *ist=NULL, *restrict i=in->array, *f=i+in->size; \ size_t s_e_ind[2]={0,iblock->size-1}; /* -1: this is INCLUSIVE */ \ \ /* If we are on a tile, the default values need to change. */ \ if(in!=iblock) \ ist=gal_tile_start_end_ind_inclusive(in, iblock, s_e_ind); \ \ /* Constant preparations before the loop. */ \ if(iblock->type==out->type) \ mclen = in==iblock ? iblock->size : contig_len; \ else \ { \ gal_blank_write(&ob, out->type); \ gal_blank_write(&ib, iblock->type); \ } \ \ /* Parse over the input and copy it. */ \ while( s_e_ind[0] + increment <= s_e_ind[1] ) \ { \ /* If we are on a tile, reset `i' and `f' for each round. */ \ if(in!=iblock) \ f = ( i = ist + increment ) + contig_len; \ \ /* When the types are the same just use memcopy, otherwise, */ \ /* We'll have to read each number (and use internal */ \ /* conversion). */ \ if(iblock->type==out->type) \ { \ memcpy(o, i, mclen*gal_type_sizeof(iblock->type)); \ o += mclen; \ } \ else \ { \ /* If the blank is a NaN value (only for floating point */ \ /* types), it will fail any comparison, so we'll exploit */ \ /* this property in such cases. For other cases, a */ \ /* `*i==ib' is enough. */ \ if(ib==ib) do *o++ = *i==ib ? ob : *i; while(++isize \ : gal_tile_block_increment(iblock, in->dsize, \ num_increment++, \ NULL) ); \ } \ } /* gal_data_copy_to_new_type: Output type is set, now choose the input type. */ #define COPY_OT_SET(OT) \ switch(iblock->type) \ { \ case GAL_TYPE_UINT8: COPY_OT_IT_SET(OT, uint8_t ); break; \ case GAL_TYPE_INT8: COPY_OT_IT_SET(OT, int8_t ); break; \ case GAL_TYPE_UINT16: COPY_OT_IT_SET(OT, uint16_t ); break; \ case GAL_TYPE_INT16: COPY_OT_IT_SET(OT, int16_t ); break; \ case GAL_TYPE_UINT32: COPY_OT_IT_SET(OT, uint32_t ); break; \ case GAL_TYPE_INT32: COPY_OT_IT_SET(OT, int32_t ); break; \ case GAL_TYPE_UINT64: COPY_OT_IT_SET(OT, uint64_t ); break; \ case GAL_TYPE_INT64: COPY_OT_IT_SET(OT, int64_t ); break; \ case GAL_TYPE_FLOAT32: COPY_OT_IT_SET(OT, float ); break; \ case GAL_TYPE_FLOAT64: COPY_OT_IT_SET(OT, double ); break; \ case GAL_TYPE_STRING: data_copy_from_string(in, out); break; \ case GAL_TYPE_BIT: \ case GAL_TYPE_STRLL: \ case GAL_TYPE_COMPLEX32: \ case GAL_TYPE_COMPLEX64: \ error(EXIT_FAILURE, 0, "%s: copying from %s type to a numeric " \ "(real) type not supported", "COPY_OT_SET", \ gal_type_name(in->type, 1)); \ break; \ \ default: \ error(EXIT_FAILURE, 0, "%s: type code %d not recognized for " \ "`in->type'", "COPY_OT_SET", in->type); \ } /* Wrapper for `gal_data_copy_to_new_type', but will copy to the same type as the input. Recall that if the input is a tile (a part of the input, which is not-contiguous if it has more than one dimension), then the output will have only the elements that cover the tile.*/ gal_data_t * gal_data_copy(gal_data_t *in) { return gal_data_copy_to_new_type(in, gal_tile_block(in)->type); } /* Copy a given data structure to a new one with any type (for the output). The input can be a tile, in which case the output will be a contiguous patch of memory that has all the values within the input tile in the requested type. */ gal_data_t * gal_data_copy_to_new_type(gal_data_t *in, uint8_t newtype) { gal_data_t *out; /* Allocate the output datastructure. */ out=gal_data_alloc(NULL, newtype, in->ndim, in->dsize, in->wcs, 0, in->minmapsize, in->name, in->unit, in->comment); /* Fill in the output array: */ gal_data_copy_to_allocated(in, out); /* Return the created array */ return out; } /* Copy the input data structure into a new type and free the allocated space. */ gal_data_t * gal_data_copy_to_new_type_free(gal_data_t *in, uint8_t newtype) { gal_data_t *out, *iblock=gal_tile_block(in); /* In a general application, it might happen that the type is equal with the type of the input and the input isn't a tile. Since the job of this function is to free the input dataset, and the user just wants one dataset after this function finishes, we can safely just return the input. */ if(newtype==iblock->type && in==iblock) return in; else { out=gal_data_copy_to_new_type(in, newtype); if(iblock==in) gal_data_free(in); else fprintf(stderr, "#####\nWarning from " "`gal_data_copy_to_new_type_free'\n#####\n The input " "dataset is a tile, not a contiguous (fully allocated) " "patch of memory. So it has not been freed. Please use " "`gal_data_copy_to_new_type' to avoid this warning.\n" "#####"); return out; } } /* Copy a given dataset (`in') into an already allocated dataset `out' (the actual dataset and its `array' element). The meta-data of `in' (except for `block') will be fully copied into `out' also. `out->size' will be used to find the available space in the allocated space. When `in->size != out->size' this function will behave as follows: `out->size < in->size': it won't re-allocate the necessary space, it will abort with an error, so please check before calling this function. `out->size > in->size': it will update `out->size' and `out->dsize' to be the same as the input. So if you want to re-use a pre-allocated space with varying input sizes, be sure to reset `out->size' before every call to this function. */ void gal_data_copy_to_allocated(gal_data_t *in, gal_data_t *out) { gal_data_t *iblock=gal_tile_block(in); /* Make sure the number of allocated elements (of whatever type) in the output is not smaller than the input. Note that the type is irrelevant because we will be doing type conversion if they differ.*/ if( out->size < in->size ) error(EXIT_FAILURE, 0, "%s: the output dataset must be equal or larger " "than the input. the sizes are %zu and %zu respectively", __func__, out->size, in->size); if( out->ndim != in->ndim ) error(EXIT_FAILURE, 0, "%s: the output dataset must have the same number " "of dimensions, the dimensions are %zu and %zu respectively", __func__, out->ndim, in->ndim); /* Write the basic meta-data. */ out->flag = in->flag; out->next = in->next; out->status = in->status; out->disp_width = in->disp_width; out->disp_precision = in->disp_precision; /* Do the copying. */ switch(out->type) { case GAL_TYPE_UINT8: COPY_OT_SET( uint8_t ); break; case GAL_TYPE_INT8: COPY_OT_SET( int8_t ); break; case GAL_TYPE_UINT16: COPY_OT_SET( uint16_t ); break; case GAL_TYPE_INT16: COPY_OT_SET( int16_t ); break; case GAL_TYPE_UINT32: COPY_OT_SET( uint32_t ); break; case GAL_TYPE_INT32: COPY_OT_SET( int32_t ); break; case GAL_TYPE_UINT64: COPY_OT_SET( uint64_t ); break; case GAL_TYPE_INT64: COPY_OT_SET( int64_t ); break; case GAL_TYPE_FLOAT32: COPY_OT_SET( float ); break; case GAL_TYPE_FLOAT64: COPY_OT_SET( double ); break; case GAL_TYPE_STRING: data_copy_to_string(in, out); break; case GAL_TYPE_BIT: case GAL_TYPE_STRLL: case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: error(EXIT_FAILURE, 0, "%s: copying to %s type not yet supported", __func__, gal_type_name(out->type, 1)); break; default: error(EXIT_FAILURE, 0, "%s: type %d not recognized for `out->type'", __func__, out->type); } /* Correct the sizes of the output to be the same as the input. If it is equal, there is no problem, if not, the size information will be changed, so if you want to use this allocated space again, be sure to re-set the size parameters. */ out->size=in->size; memcpy(out->dsize, in->dsize, in->ndim * sizeof *(in->dsize) ); } /* Just a wrapper around `gal_type_from_string_auto', to return a `gal_data_t' dataset hosting the allocated number. */ gal_data_t * gal_data_copy_string_to_number(char *string) { void *ptr; uint8_t type; size_t dsize=1; ptr=gal_type_string_to_number(string, &type); return ( ptr ? gal_data_alloc(ptr, type, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL) : NULL ); } gnuastro-0.5/lib/cosmology.c0000644000175000017500000001770313173367042013104 00000000000000/********************************************************************* Cosmological calculations. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /**************************************************************/ /************ Definitions *************/ /**************************************************************/ /* These are basic definitions that commonly go into the header files. But because this is a library and the user imports the header file, it is easier to just have them here in the main C file to avoid filling up the user's name-space with junk. */ struct cosmology_integrand_t { double o_lambda_0; double o_curv_0; double o_matter_0; double o_radiation_0; }; /* For the GSL integrations */ #define GSLILIMIT 1000 #define GSLIEPSABS 0 #define GSLIEPSREL 1e-7 /**************************************************************/ /************ Integrand functions *************/ /**************************************************************/ /* These are integrands, they won't be giving the final value. */ static double cosmology_integrand_Ez(double z, void *params) { struct cosmology_integrand_t *p=(struct cosmology_integrand_t *)params; return sqrt( p->o_lambda_0 + p->o_curv_0 * (1+z) * (1+z) + p->o_matter_0 * (1+z) * (1+z) * (1+z) + p->o_radiation_0 * (1+z) * (1+z) * (1+z) * (1+z)); } static double cosmology_integrand_age(double z, void *params) { return 1 / ( (1.0 + z) * cosmology_integrand_Ez(z,params) ); } static double cosmology_integrand_proper_dist(double z, void *params) { return 1 / ( cosmology_integrand_Ez(z,params) ); } static double cosmology_integrand_comoving_volume(double z, void *params) { size_t neval; gsl_function F; double result, error; /* Set the GSL function parameters */ F.params=params; F.function=&cosmology_integrand_proper_dist; gsl_integration_qng(&F, 0.0, z, GSLIEPSABS, GSLIEPSREL, &result, &error, &neval); return result * result / ( cosmology_integrand_Ez(z,params) ); } /**************************************************************/ /************ Final functions *************/ /**************************************************************/ /* Age of the universe (in Gyrs). H0 is in units of (km/sec/Mpc) and the fractional densities must add up to 1. */ double gal_cosmology_age(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { gsl_function F; double result, error; double o_curv_0 = 1.0 - ( o_lambda_0 + o_matter_0 + o_radiation_0 ); double H0s=H0/1000/GSL_CONST_MKSA_PARSEC; /* H0 in units of seconds. */ gsl_integration_workspace *w=gsl_integration_workspace_alloc(GSLILIMIT); struct cosmology_integrand_t p={o_lambda_0, o_curv_0, o_matter_0, o_radiation_0}; /* Set the GSL function parameters. */ F.params=&p; F.function=&cosmology_integrand_age; gsl_integration_qagiu(&F, z, GSLIEPSABS, GSLIEPSREL, GSLILIMIT, w, &result, &error); return result / H0s / (365*GSL_CONST_MKSA_DAY) / 1e9; } /* Proper distance to z (Mpc). */ double gal_cosmology_proper_distance(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { size_t neval; gsl_function F; double result, error, c=GSL_CONST_MKSA_SPEED_OF_LIGHT; double o_curv_0 = 1.0 - ( o_lambda_0 + o_matter_0 + o_radiation_0 ); double H0s=H0/1000/GSL_CONST_MKSA_PARSEC; /* H0 in units of seconds. */ struct cosmology_integrand_t p={o_lambda_0, o_curv_0, o_matter_0, o_radiation_0}; /* Set the GSL function parameters */ F.params=&p; F.function=&cosmology_integrand_proper_dist; /* Do the integration. */ gsl_integration_qng(&F, 0.0f, z, GSLIEPSABS, GSLIEPSREL, &result, &error, &neval); /* Return the result. */ return result * c / H0s / (1e6 * GSL_CONST_MKSA_PARSEC); } /* Comoving volume over 4pi stradian to z (Mpc^3). */ double gal_cosmology_comoving_volume(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { size_t neval; gsl_function F; double result, error; double c=GSL_CONST_MKSA_SPEED_OF_LIGHT; double H0s=H0/1000/GSL_CONST_MKSA_PARSEC; /* H0 in units of seconds. */ double cH = c / H0s / (1e6 * GSL_CONST_MKSA_PARSEC); double o_curv_0 = 1.0 - ( o_lambda_0 + o_matter_0 + o_radiation_0 ); struct cosmology_integrand_t p={o_lambda_0, o_curv_0, o_matter_0, o_radiation_0}; /* Set the GSL function parameters */ F.params=&p; F.function=&cosmology_integrand_comoving_volume; /* Do the integration. */ gsl_integration_qng(&F, 0.0f, z, GSLIEPSABS, GSLIEPSREL, &result, &error, &neval); /* Return the result. */ return result * 4 * M_PI * cH*cH*cH; } /* Critical density at redshift z in units of g/cm^3. */ double gal_cosmology_critical_density(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { double H; double H0s=H0/1000/GSL_CONST_MKSA_PARSEC; /* H0 in units of seconds. */ double o_curv_0 = 1.0 - ( o_lambda_0 + o_matter_0 + o_radiation_0 ); struct cosmology_integrand_t p={o_lambda_0, o_curv_0, o_matter_0, o_radiation_0}; /* Set the place holder, then return the result. */ H = H0s * cosmology_integrand_Ez(z, &p); return 3*H*H/(8*M_PI*GSL_CONST_MKSA_GRAVITATIONAL_CONSTANT)/1000; } /* Angular diameter distance to z (Mpc). */ double gal_cosmology_angular_distance(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { return gal_cosmology_proper_distance(z, H0, o_lambda_0, o_matter_0, o_radiation_0) / (1+z); } /* Luminosity distance to z (Mpc). */ double gal_cosmology_luminosity_distance(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { return gal_cosmology_proper_distance(z, H0, o_lambda_0, o_matter_0, o_radiation_0) * (1+z); } /* Distance modulus at z (no units). */ double gal_cosmology_distance_modulus(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { double ld=gal_cosmology_luminosity_distance(z, H0, o_lambda_0, o_matter_0, o_radiation_0); return 5*(log10(ld*1000000)-1); } /* Convert apparent to absolute magnitude. */ double gal_cosmology_to_absolute_mag(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0) { double dm=gal_cosmology_distance_modulus(z, H0, o_lambda_0, o_matter_0, o_radiation_0); return dm-2.5*log10(1.0+z); } gnuastro-0.5/lib/convolve.c0000644000175000017500000005207013136321727012717 00000000000000/********************************************************************* Convolve -- Convolve a dataset with a given kernel. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include #include /*********************************************************************/ /******************** Utilities ********************/ /*********************************************************************/ /* See if the tile is on the edge of the hosted region or not. It doesn't matter if the host is the allocated block of memory or a region in it (a channel). */ static int convolve_tile_is_on_edge(size_t *h, size_t *start_end_coord, size_t *k, size_t ndim) { size_t *s=start_end_coord, *e=start_end_coord+ndim, *kf=k+ndim; /* If the starting point of the tile is smaller than the half-kernel length along that dimension, then the tile is on the edge. If the end of the tile in this dimension added with the half-kernel length along that dimension is equal to or larger than the host's size, then the tile is on the edge. */ do if( (*s++ < *k/2) || (*e++ + *k/2 >= *h++) ) return 1; while(++kcprm; gal_data_t *block=cprm->block, *kernel=cprm->kernel; size_t *dsize = tocorrect ? block->dsize : pprm->host->dsize; size_t ndim=block->ndim; size_t *kd=pprm->k_overlap->dsize; size_t *pp, *ppf, *hs, increment, size=1; size_t *h=dsize, *os=pprm->overlap_start; size_t *p, *pf, *od=pprm->i_overlap->dsize; size_t *k=kernel->dsize, *ks=pprm->kernel_start; int full_overlap=1, dim_full_overlap, is_start, is_end; /* In to-correct mode, the pix position needs to be relative to the block. */ if(tocorrect) { hs=pprm->host_start; ppf=(pp=pprm->pix)+ndim; do *pp += *hs++; while(++pppix) + ndim; do { /* Initialize the overlap for this dimension (we'll assume it overlaps because this is the most common case usually). */ dim_full_overlap=1; /* When the tile is on the edge, some pixels in it can have full overlap. So using the `dim_full_overlap', we will do the same thing we do for the tiles that don't overlap for them. When `tocorrect!=0', then only pixels that are on the edge of the tile will get to this point, so it must always be checked. */ if( tocorrect ? 1 : pprm->on_edge ) { /* See if this pixel is on the start and/or end of the dimension relative to the kernel. */ is_start = *p < *k/2; is_end = (*p + *k/2) >= *h; if( is_start || is_end ) { /* Overlapping with the outside. With the start: assume that in this dimension, the pixel is at position 2, while the kernel is 11 pixels wide (or 5 pixels in half-width). As seen below, the kernel should start from pixel `5-2=3' in this dimension and the overlap size should decrease by the same amount. image: 0 1 2 3 4 5 6 7 8 9 ... pixel: p kernel: 0 1 2 3 4 5 6 7 8 9 10 With the end: Similar to above, but assume the pixel is two pixels away from the edge of a 100-pixel image. We are no longer worried about the overlap or kernel starting point, it is the width that we need to decrease it by: 97 + 5 - 100 + 1 : The `1' is because we want the pixel immediately after the end. image: ... 92 93 94 95 96 97 98 99 | 100 101 102 pixel: p kernel: 0 1 2 3 4 5 6 7 8 | 9 10 */ *ks++ = is_start ? *k/2 - *p : 0; *os++ = is_start ? 0 : *p - *k/2; /* We will start with the full kernel width, then decrease it if the pixel is too close to the start or end along this dimension. Note that the host array/image might actually be smaller than kernel, so both cases might occur. */ *od = *k; if(is_start) *od -= *k/2 - *p; if(is_end) *od -= *p + *k/2 - *h + 1; /* Put the overlap size into the kernel's overlap `dsize' also and then use it to update the total size of the overlap. */ *kd++ = *od; size *= *od; /* Increment and finalize. */ ++h; ++k; ++od; full_overlap=0; dim_full_overlap=0; } } /* There is full overlap for this pixel or tile over this dimension. */ if(dim_full_overlap) { /* Set the values. */ *ks++ = 0; size *= *k; *kd++ = *od = *k; *os++ = *p - *k/2; /* Increment. */ ++h; ++k; ++od; } } while(++pi_overlap->size = pprm->k_overlap->size = size; /* Make correction. Normal mode (when `tocorrect==0'): add the host's starting location (necessary when convolution over the host/channel is treated independently). In this mode, until now we were working as if the the host/channel is the full image so the edges don't get mixed. But from now on we will be working over the allocated block to look at pixel values, so we need to convert the location to the proper place within the allocated array. To-correct mode: The boundaries were calculated with respect to the block, so we don't need to correct `overlap_start'. But we need to correct the pixel position back to its original state (relative to the channel). */ hs=pprm->host_start; if(tocorrect) { ppf=(pp=pprm->pix) + ndim; do *pp -= *hs++; while(++ppoverlap_start) + ndim; do *pp += *hs++; while(++ppdsize, pprm->overlap_start); pprm->i_overlap->array=gal_data_ptr_increment(block->array, increment, block->type); /* Set the starting point of the kernel overlap tile. */ increment = ( full_overlap ? 0 : gal_dimension_coord_to_index(ndim, kernel->dsize, pprm->kernel_start) ); pprm->k_overlap->array=gal_data_ptr_increment(kernel->array, increment, kernel->type); return full_overlap; } /* Convolve over one tile that is not touching the edge. */ static void convolve_spatial_tile(struct per_thread_spatial_prm *pprm) { gal_data_t *tile=pprm->tile; int full_overlap; double sum, ksum; struct spatial_params *cprm=pprm->cprm; gal_data_t *block=cprm->block, *kernel=cprm->kernel; size_t j, ndim=block->ndim, csize=tile->dsize[ndim-1]; gal_data_t *i_overlap=pprm->i_overlap, *k_overlap=pprm->k_overlap; /* Variables for scanning a tile (`i_*') and the region around every pixel of a tile (`o_*'). */ size_t start_fastdim; size_t i_inc, i_ninc, i_st_en[2]; /* These variables depend on the type of the input. */ float *i_start; float *in_v, *in=block->array, *out=cprm->out->array; /* Starting pixel for the host of this tile. Note that when we are in `convoverch' mode, `host' refers to the fully allocated block of memory. */ pprm->host=cprm->convoverch ? block : tile->block; gal_tile_start_coord(pprm->host, pprm->host_start); /* Set the starting and ending coordinates of this tile (recall that the space for the start and end coordinates is stored in `p->pix'). When `convoverch' is set, we want to convolve over the whole allocated block, not just one channel. So in effect, it is the same as `rel_block' in `gal_tile_start_end_coord'. */ gal_tile_start_end_coord(tile, pprm->pix, cprm->convoverch); start_fastdim = pprm->pix[ndim-1]; /* See if this tile is on the edge or not. */ pprm->on_edge=convolve_tile_is_on_edge(pprm->host->dsize, pprm->pix, kernel->dsize, ndim); /* If it isn't on the edge and we are correcting an already convolved image (`tocorrect!=NULL'), then this tile can be ignored. */ if(cprm->tocorrect && pprm->on_edge==0) return; /* Parse over all the tile elements. */ i_inc=0; i_ninc=1; i_start=gal_tile_start_end_ind_inclusive(tile, block, i_st_en); while( i_st_en[0] + i_inc <= i_st_en[1] ) { /* Initialize the value along the fastest dimension (it is not incremented during `gal_tile_block_increment'). */ pprm->pix[ndim-1]=start_fastdim; /* Go over each pixel to convolve. */ for(j=0;jtocorrect && full_overlap) ) { /* If we are in correct mode, then re-calculate the full-overlap and all the other necessary paramters as if the channels didn't exist. */ if(cprm->tocorrect) full_overlap=convolve_spatial_overlap(pprm, 1); /* Initialize the necessary values. */ sum = 0.0L; ksum = cprm->edgecorrection ? 0.0L : 1.0L; /* Parse over both the overlap tiles. */ GAL_TILE_PO_OISET(float, float, i_overlap, k_overlap, 1, 0, { if( !isnan(*i) ) { sum += *i * *o; if(cprm->edgecorrection) ksum += *o; } }); /* Set the output value. */ out[ in_v - in ] = ksum==0.0L ? NAN : sum/ksum; } } /* Increment the last coordinate. */ pprm->pix[ndim-1]++; } /* Increase the increment from the start of the tile for the next contiguous patch. */ i_inc += gal_tile_block_increment(block, tile->dsize, i_ninc++, pprm->pix); } /* if(pprm->id==2053) printf("... done.\n"); */ } /* Do spatial convolution on each mesh. */ static void * convolve_spatial_on_thread(void *inparam) { struct gal_threads_params *tprm=(struct gal_threads_params *)inparam; struct spatial_params *cprm=(struct spatial_params *)(tprm->params); gal_data_t *block=cprm->block; size_t i; size_t ndim=block->ndim; struct per_thread_spatial_prm *pprm=&cprm->pprm[tprm->id]; size_t *dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "dsize"); /* Set all dsize values to 1 (the values within `overlap->dsize' will be changed during convolution). */ for(i=0;icprm = cprm; pprm->pix = gal_data_malloc_array(GAL_TYPE_SIZE_T, 2*ndim, __func__, "pprm->pix"); pprm->host_start = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "pprm->host_start"); pprm->kernel_start = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "pprm->kernel_start"); pprm->overlap_start = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "pprm->overlap_start"); pprm->i_overlap = gal_data_alloc(NULL, block->type, ndim, dsize, NULL, 0, -1, NULL, NULL, NULL); pprm->k_overlap = gal_data_alloc(NULL, cprm->kernel->type, ndim, dsize, NULL, 0, -1, NULL, NULL, NULL); free(dsize); free(pprm->i_overlap->array); free(pprm->k_overlap->array); pprm->i_overlap->block = cprm->block; pprm->k_overlap->block = cprm->kernel; /* Go over all the tiles given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* Set this tile's pointer into this thread's parameters. */ pprm->id = tprm->indexs[i]; pprm->tile = &cprm->tiles[ pprm->id ]; /* Do the convolution on this tile. */ convolve_spatial_tile(pprm); } /* Clean up, wait until all other threads finish, then return. In a single thread situation, `tprm->b==NULL'. */ free(pprm->pix); free(pprm->host_start); free(pprm->kernel_start); free(pprm->overlap_start); gal_data_free(pprm->i_overlap); gal_data_free(pprm->k_overlap); if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* General spatial convolve function. This function is called by both `gal_convolve_spatial' and */ static gal_data_t * gal_convolve_spatial_general(gal_data_t *tiles, gal_data_t *kernel, size_t numthreads, int edgecorrection, int convoverch, gal_data_t *tocorrect) { struct spatial_params params; gal_data_t *out, *block=gal_tile_block(tiles); /* Small sanity checks. */ if(tiles->ndim!=kernel->ndim) error(EXIT_FAILURE, 0, "%s: The number of dimensions between the kernel " "and input should be the same", __func__); if( block->type!=GAL_TYPE_FLOAT32 || kernel->type!=GAL_TYPE_FLOAT32 ) error(EXIT_FAILURE, 0, "%s: only accepts `float32' type input and " "kernel currently", __func__); /* Set the output datastructure. */ if(tocorrect) out=tocorrect; else { /* Allocate the space for the convolved image. */ out=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, block->ndim, block->dsize, block->wcs, 0, block->minmapsize, NULL, block->unit, NULL); /* Spatial convolution won't change the blank bit-flag, so use the block structure's blank bit flag. */ out->flag = ( block->flag | ( GAL_DATA_FLAG_BLANK_CH | GAL_DATA_FLAG_HASBLANK ) ); } /* Set the pointers in the parameters structure. */ params.out=out; params.tiles=tiles; params.block=block; params.kernel=kernel; params.tocorrect=tocorrect; params.convoverch=convoverch; params.edgecorrection=edgecorrection; /* Allocate the per-thread parameters. */ errno=0; params.pprm=malloc(numthreads * sizeof *params.pprm); if(params.pprm==NULL) error(EXIT_FAILURE, 0, "%s: %zu bytes for `params.pprm'", __func__, numthreads * sizeof *params.pprm); /* Do the spatial convolution on threads. */ gal_threads_spin_off(convolve_spatial_on_thread, ¶ms, gal_list_data_number(tiles), numthreads); /* Clean up and return the output array. */ free(params.pprm); return out; } /* Convolve a dataset with a given kernel in the spatial domain. Spatial convolution can be greatly sped up if it is done on separate tiles over the image (on multiple threads). So as input, you can either give tile values or one full array. Just note that if you give a single array as input, the `next' element has to be `NULL'.*/ gal_data_t * gal_convolve_spatial(gal_data_t *tiles, gal_data_t *kernel, size_t numthreads, int edgecorrection, int convoverch) { /* Call the general function. */ return gal_convolve_spatial_general(tiles, kernel, numthreads, edgecorrection, convoverch, NULL); } /* Correct the edges of channels in an already convolved image when it was initially convolved with `gal_convolve_spatial' with `convoverch==0'. In that case, strong boundaries exist on the tile edges. So if you later need to remove those boundaries, you can call this function, it will only do convolution on the tiles that are near the edge, not the full area, so it is much faster. */ void gal_convolve_spatial_correct_ch_edge(gal_data_t *tiles, gal_data_t *kernel, size_t numthreads, int edgecorrection, gal_data_t *tocorrect) { gal_data_t *block=gal_tile_block(tiles); /* Some small sanity checks. */ if( gal_data_dsize_is_different(block, tocorrect) ) error(EXIT_FAILURE, 0, "%s: the `tocorrect' dataset has to have the " "same dimensions/size as the block of the `tiles' input", __func__); if( block->type != tocorrect->type ) error(EXIT_FAILURE, 0, "%s: the `tocorrect' dataset has to have the same " "type as the block of the `tiles' input. The given types are `%s' " "and `%s' respectively", __func__, gal_type_name(tocorrect->type, 1), gal_type_name(block->type, 1)); /* Call the general function, which will do the correction. */ gal_convolve_spatial_general(tiles, kernel, numthreads, edgecorrection, 0, tocorrect); } gnuastro-0.5/lib/checkset.c0000644000175000017500000003521513211076737012661 00000000000000/********************************************************************* Functions to check and set command line argument values and files. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /**************************************************************/ /********** My String functions: ************/ /**************************************************************/ int gal_checkset_string_has_space(char *in) { do switch(*in) { case ' ': case '\t': case '\v': return 1; } while(*(++in)!='\0'); return 0; } char * gal_checkset_malloc_cat(char *inname, char *toappend) { char *out; size_t inl, apl; inl=strlen(inname); apl=strlen(toappend); errno=0; out=malloc(inl+apl+1); if(out==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes", __func__, inl+apl+1); strcpy(out, inname); strcat(out, toappend); return out; } /* Copy the input string to the output (and also allocate the output. */ void gal_checkset_allocate_copy(const char *arg, char **copy) { if(arg) { errno=0; *copy=malloc(strlen(arg)+1); if(*copy==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes to copy %s", __func__, strlen(arg)+1, arg); strcpy(*copy, arg); } else *copy=NULL; } /* This function is mainly for reading in the arguments (from the command line or configuration files) that need to be copied. The set argument is for making sure that it has not already been set before, see the main.h files of any program. */ void gal_checkset_allocate_copy_set(char *arg, char **copy, int *set) { /* Incase *set==1, then you shouldn't do anything, just return. */ if(*set) return; /* The variable was not copied, copy it: */ errno=0; *copy=malloc(strlen(arg)+1); if(*copy==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes to copy %s", __func__, strlen(arg)+1, arg); strcpy(*copy, arg); *set=1; } /* The dataset may be alone in a file (for example a table in a text file) or it may an extension of a FITS file. In error messages in particular, we need to differentiate between the two. This function will check the filename and if it is FITS, it will return a string with the filename and HDU in parenthesis. If it isn't a FITS file, it will only return the filename. Note that the output needs to be freed, although when used in an error message, you can leave it to the system to free the space. There is no problem. */ char * gal_checkset_dataset_name(char *filename, char *hdu) { char *out; if( gal_fits_name_is_fits(filename) ) asprintf(&out, "%s (hdu %s)", filename, hdu); else gal_checkset_allocate_copy(filename, &out); return out; } /**************************************************************/ /********** Set file names and check if they exist ************/ /**************************************************************/ /* Given a filename, this function will separate its directory name part. */ char * gal_checkset_dir_part(char *filename) { char *out; size_t i, l=strlen(filename); /* Find the first slash from the end. */ for(i=l;i!=0;--i) if(filename[i]=='/') break; /* If there was no slash, then the current directory should be given: */ if(i==0 && filename[0]!='/') gal_checkset_allocate_copy("./", &out); else { gal_checkset_allocate_copy(filename, &out); out[i+1]='\0'; } return out; } /* Given a file name, keep the non-directory part. Note that if there is no forward slash in the input name, the full input name is considered to be the notdir output.*/ char * gal_checkset_not_dir_part(char *filename) { size_t i, l; char *out, *tmp=filename; /* Find the first `/' to identify the directory */ l=strlen(filename); for(i=l;i!=0;--i) if(filename[i]=='/') { tmp=&filename[i+1]; break; } /* Get the length of the notdir name: */ l=strlen(tmp); errno=0; out=malloc((l+1)*sizeof *out); if(out==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for notdir", __func__, (l+1)*sizeof *out); strcpy(out, tmp); return out; } /* Check if a file exists and report if it doesn't: */ void gal_checkset_check_file(char *filename) { FILE *tmpfile; errno=0; tmpfile = fopen(filename, "r"); if(tmpfile) /* The file opened. */ { if(fclose(tmpfile)==EOF) error(EXIT_FAILURE, errno, "%s", filename); } else error(EXIT_FAILURE, errno, "%s", filename); } /* Similar to `gal_checkset_check_file', but will report the result instead of doing it quietly. */ int gal_checkset_check_file_return(char *filename) { FILE *tmpfile; errno=0; tmpfile = fopen(filename, "r"); if(tmpfile) /* The file opened. */ { if(fclose(tmpfile)==EOF) error(EXIT_FAILURE, errno, "%s", filename); return 1; } else return 0; } /* Check if a file exists and can be opened. If the `keep' value is non-zero, then the file will remain untouched, otherwise, it will be deleted (since most programs need to make a clean output). When the file is to be deleted and `dontdelete' has a non-zero value, then the file won't be deleted, but the program will abort with an error, informing the user that the output can't be made. */ void gal_checkset_writable_remove(char *filename, int keep, int dontdelete) { char *dir; FILE *tmpfile; /* If the filename is `NULL' everything is ok (it doesn't exist)! In some cases, a NULL filename is interpretted to mean standard output. */ if(filename==NULL) return; /* We want to make sure that we can open and write to this file. But the user might have asked to not delete the file, so the contents should not be changed. Therefore we have to open it with `r+`. */ errno=0; tmpfile=fopen(filename, "r+"); if (tmpfile) /* The file opened. */ { /* Close the file. */ errno=0; if(fclose(tmpfile)) error(EXIT_FAILURE, errno, "%s", filename); /* See if the file should be deleted. */ if(keep==0) { /* Make sure it is ok to delete the file. */ if(dontdelete) error(EXIT_FAILURE, 0, "%s already exists and you have " "asked to not remove it with the `--dontdelete` " "(`-D`) option", filename); /* Delete the file: */ errno=0; if(unlink(filename)) error(EXIT_FAILURE, errno, "%s", filename); } } /* If the file doesn't exist, we just need to make sure if we have write permissions to its host directory. */ else { /* Separate the directory part of the filename. */ dir=gal_checkset_dir_part(filename); /* Make sure this directory is writable by this user. */ errno=0; if( access(dir, W_OK) ) error(EXIT_FAILURE, errno, "cannot create any file(s) in the " "directory `%s'", dir); /* Clean up. */ free(dir); } } /* Check output file name: If a file exists or can exist and can be written to, this function will return 1. If not (for example it is a directory) it will return 0. Finally, if it exists but cannot be deleted, report an error and abort. */ int gal_checkset_dir_0_file_1(char *name, int dontdelete) { FILE *tmpfile; struct stat nameinfo; if(name==NULL) error(EXIT_FAILURE, 0, "%s: a bug! The input should not be NULL. " "Please contact us at %s so we can see what went wrong and " "fix it in future updates", __func__, PACKAGE_BUGREPORT); errno=0; if(stat(name, &nameinfo)!=0) { if(errno==ENOENT) /* ENOENT: No such file or directory. */ {/* Make the file temporarily and see if everything is ok. */ errno=0; tmpfile=fopen(name, "w"); if (tmpfile) { fprintf(tmpfile, "Only to test write access."); errno=0; if(fclose(tmpfile)) error(EXIT_FAILURE, errno, "%s", name); errno=0; if(unlink(name)) error(EXIT_FAILURE, errno, "%s", name); } else error(EXIT_FAILURE, errno, "%s", name); return 1; /* It is a file name, GOOD */ } else /* Some strange condition, ABORT */ error(EXIT_FAILURE, errno, "%s", name); } if(S_ISDIR(nameinfo.st_mode)) /* It is a directory, BAD */ return 0; else if (S_ISREG(nameinfo.st_mode)) /* It is a file, GOOD. */ { gal_checkset_writable_remove(name, 0, dontdelete); return 1; } else /* Not a file or a dir, ABORT */ error(EXIT_FAILURE, 0, "%s not a file or a directory", name); error(EXIT_FAILURE, 0, "%s: a bug! The process should not reach the end " "of the function! Please contact us at %s so we can see what went " "wrong and fix it in future updates", __func__, PACKAGE_BUGREPORT); return 0; } /* Allocate space and write the output name (outname) based on a given input name (inname). The suffix of the input name (if present) will be removed and the given suffix will be put in the end. */ char * gal_checkset_automatic_output(struct gal_options_common_params *cp, char *inname, char *suffix) { char *out; size_t i, l, offset=0; /* Merge the contents of the input name and suffix name (while also allocating the necessary space).*/ out=gal_checkset_malloc_cat(inname, suffix); /* If there is actually a suffix, replace it with the (possibly) existing suffix. */ if(suffix) { /* Start from the end of the input array*/ l=strlen(inname); for(i=l-1;i!=0;--i) { /* We don't want to touch anything before a `/' (directory names). We are only concerned with file names here. */ if(out[i]=='/') { /* When `/' is the last input character, then the input is clearly not a filename, but a directory name. In this case, adding a suffix is meaningless (a suffix belongs to a filename for Gnuastro's tools). So close the string after the `/' and leave the loop. However, if the `/' isn't the last input name charector, there is probably a filename (without a "." suffix), so break from the loop. No further action is required, since we initially allocated the necessary space and concatenated the input and suffix arrays. */ if(i==l-1) out[i+1]='\0'; break; } /* The input file names can be compressed names (for example `.fits.gz'). Currently the only compressed formats (decompressed within CFITSIO) are listed in `gal_fits_name_is_fits' and `gal_fits_suffix_is_fits'.*/ else if(out[i]=='.' && !( ( out[i+1]=='g' && out[i+2]=='z' ) || (out[i+1]=='f' && out[i+2]=='z' ) || out[i+1]=='Z' ) ) { out[i]='\0'; strcat(out, suffix); break; } } } /* If we don't want the input directory information, remove them here. */ if(!cp->keepinputdir) { l=strlen(out); for(i=l;i!=0;--i) /* Find the last forward slash. */ if(out[i]=='/') {offset=i+1; break;} if(offset) for(i=offset;i<=l;++i) /* <= because we want to shift the */ out[i-offset]=out[i]; /* '\0' character in the string too. */ } /* Remove the created filename if it already exits. */ gal_checkset_writable_remove(out, cp->keep, cp->dontdelete); /* Return the resulting filename. */ return out; } /* Check if dirname is actually a real directory and that we can actually write inside of it. To insure all conditions an actual file will be made */ void gal_checkset_check_dir_write_add_slash(char **dirname) { int file_d; char *tmpname, *indir=*dirname/*, buf[]="A test"*/; /* Set the template for the temporary file: */ if(indir[strlen(indir)-1]=='/') tmpname=gal_checkset_malloc_cat(indir, "gnuastroXXXXXX"); else tmpname=gal_checkset_malloc_cat(indir, "/gnuastroXXXXXX"); /* Make a temporary file name and try openning it. */ errno=0; file_d=mkstemp(tmpname); if(file_d==-1) error(EXIT_FAILURE, errno, "cannot write output in the directory " "%s", indir); /* errno=0; printf("\n\n%s\n\n", tmpname); if( write(file_d, buf, strlen(buf)) == -1 ) error(EXIT_FAILURE, errno, "%s: writing to this temporary file to " "check the given `%s` directory", tmpname, indir); */ errno=0; if( close(file_d) == -1 ) error(EXIT_FAILURE, errno, "%s: Closing this temporary file to check " "the given `%s` directory", tmpname, indir); /* Delete the temporary file: */ errno=0; if(unlink(tmpname)==-1) error(EXIT_FAILURE, errno, "%s: removing this temporary file made " "to check the given `%s directory`", tmpname, indir); /* Remove the extra characters that were added for the random name. */ tmpname[strlen(tmpname)-14]='\0'; free(*dirname); *dirname=tmpname; } /* If the given directory exists, then nothing is done, if it doesn't, it will be created. */ void gal_checkset_mkdir(char *dirname) { struct stat st={0}; if( stat(dirname, &st) == -1 ) { errno=0; if( mkdir(dirname, 0700) == -1 ) error(EXIT_FAILURE, errno, "making %s", dirname); } } gnuastro-0.5/lib/box.c0000644000175000017500000002342713216276304011657 00000000000000/********************************************************************* Box -- Define bounding and overlapping boxes. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* IMPORTANT NOTE: All the axises are based on the FITS standard, not C. */ /* Any ellipse can be enclosed into a rectangular box. The purpose of this function is to give the height and width of that box. The logic behind it is this: All the points on the circumference of an ellipse that is aligned on the x axis can be written as: (acos(t),bsin(t)) where 0=0.5 ? 1 : 0 ); /* Set the first and last pixels in this dimension. */ fpixel[i]=tmp-width[i]/2; lpixel[i]=tmp+width[i]/2; } /* For a check: if(ndim==2) { printf("center: %g, %g\n", center[0], center[1]); printf("fpixel: %ld, %ld\n", fpixel[0], fpixel[1]); printf("lpixel: %ld, %ld\n", lpixel[0], lpixel[1]); } else if(ndim==3) { printf("center: %g, %g, %g\n", center[0], center[1], center[2]); printf("fpixel: %ld, %ld, %ld\n", fpixel[0], fpixel[1], fpixel[2]); printf("lpixel: %ld, %ld, %ld\n", lpixel[0], lpixel[1], lpixel[2]); } */ } /* Problem to solve: We have set the first and last pixels of a box in an input image (fpixel_i[2] and lpixel_i[2]). But those first and last pixels don't necessarily lie within the image's boundaries. They can be outside of it or patially overlap with it (see examples below). The job of this function is to corret for such situations and find the starting and ending points of any overlap. It is assumed that your output (overlap) image's first pixel lies right ontop of the fpixel_i[0] in the input image. But since fpixel_i might be outside of the image, in this function we find the fpixel_o[2] and lpixel_o[2] in the overlap image coordinates that overlap with the input image. So the values of all four points might change after this function. Before: ======= fpixel_o and lpixel_o are not shown. fpixel_o and lpixel_o point to the same place as fpixel_i and lpixel_i, But in the coordinates of the overlap image. -----------------lpixel_i | overlap | | image | | | ----------------------|------ | | | | | | fpixel_i ----------------- | | | | | | | Input image | ----------------------------- After ===== ----------------- | overlap | | image | | | ----------------------|------lpixel_i | | | | | | fpixel_i ----------------- | | | | | | | Input image | ----------------------------- So, in short the arrays we are dealing with here are: fpixel_i: Coordinates of the first pixel in input image. lpixel_i: Coordinates of the last pixel in input image. fpixel_o: Coordinates of the first pixel in overlap image. lpixel_o: Coordinates of the last pixel in overlap image. NOTES: ====== - lpixel is the last pixel in the image (not outside of it). - The coordinates are in the FITS format. Return value: ============= 1: There is an overlap 0: There is no overlap */ int gal_box_overlap(long *naxes, long *fpixel_i, long *lpixel_i, long *fpixel_o, long *lpixel_o, size_t ndim) { size_t i; long width; /* In case you want to see how things are going: printf("\n\nImage size: ["); for(i=0;inaxes[i]) { lpixel_o[i] = width - (lpixel_i[i]-naxes[i]); lpixel_i[i] = naxes[i]; } } /* In case you want to see the results. printf("\nAfter correction:\n"); printf("Input image: ("); for(i=0;inaxes[i] || lpixel_i[i]<1 ) return 0; /* The first and last image pixels are within the image, so there is overlap. */ return 1; } gnuastro-0.5/lib/blank.c0000644000175000017500000004101113156610402012135 00000000000000/********************************************************************* blank -- Deal with blank values in a datasets This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /* Write the blank value of the type into an already allocate space. Note that for STRINGS, pointer should actually be `char **'. */ void gal_blank_write(void *ptr, uint8_t type) { switch(type) { /* Numeric types */ case GAL_TYPE_UINT8: *(uint8_t *)ptr = GAL_BLANK_UINT8; break; case GAL_TYPE_INT8: *(int8_t *)ptr = GAL_BLANK_INT8; break; case GAL_TYPE_UINT16: *(uint16_t *)ptr = GAL_BLANK_UINT16; break; case GAL_TYPE_INT16: *(int16_t *)ptr = GAL_BLANK_INT16; break; case GAL_TYPE_UINT32: *(uint32_t *)ptr = GAL_BLANK_UINT32; break; case GAL_TYPE_INT32: *(int32_t *)ptr = GAL_BLANK_INT32; break; case GAL_TYPE_UINT64: *(uint64_t *)ptr = GAL_BLANK_UINT64; break; case GAL_TYPE_INT64: *(int64_t *)ptr = GAL_BLANK_INT64; break; case GAL_TYPE_FLOAT32: *(float *)ptr = GAL_BLANK_FLOAT32; break; case GAL_TYPE_FLOAT64: *(double *)ptr = GAL_BLANK_FLOAT64; break; /* String type. */ case GAL_TYPE_STRING: gal_checkset_allocate_copy(GAL_BLANK_STRING, ptr); break; /* Complex types */ case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: error(EXIT_FAILURE, 0, "%s: complex types are not yet supported", __func__); /* Unrecognized type. */ default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } } /* Allocate some space for the given type and put the blank value into it. */ void * gal_blank_alloc_write(uint8_t type) { void *out; /* Allocate the space to keep the blank value. */ out=gal_data_malloc_array(type, 1, __func__, "out"); /* Put the blank value in the allcated space. */ gal_blank_write(out, type); /* Return the allocated space. */ return out; } /* Initialize (set all the values in the array) with the blank value of the given type. */ void gal_blank_initialize(gal_data_t *input) { GAL_TILE_PARSE_OPERATE(input, NULL, 0, 0, {*i=b;}); } /* Return 1 if the dataset has a blank value and zero if it doesn't. Before checking the dataset, this function will look at its flags. If the `GAL_DATA_FLAG_HASBLANK' or `GAL_DATA_FLAG_DONT_CHECK_ZERO' bits of `input->flag' are set to 1, this function will not do any check and will just use the information in the flags. If you want to re-check a dataset which has non-zero flags, then explicitly set the appropriate flag to zero before calling this function. When there are no other flags, you can just set `input->flags' to zero, otherwise you can use this expression: input->flags &= ~ (GAL_DATA_FLAG_HASBLANK | GAL_DATA_FLAG_USE_ZERO); This function has no side-effects on the dataset: it will not toggle the flags, to avoid repeating parsing of the full dataset multiple times (when it occurs), please toggle the flags your self after the first check. */ #define HAS_BLANK(IT) { \ IT b, *a=input->array, *af=a+input->size, *start; \ gal_blank_write(&b, block->type); \ \ /* If this is a tile, not a full block. */ \ if(input!=block) \ start=gal_tile_start_end_ind_inclusive(input, block, start_end_inc); \ \ /* Go over all the elements. */ \ while( start_end_inc[0] + increment <= start_end_inc[1] ) \ { \ /* Necessary when we are on a tile. */ \ if(input!=block) \ af = ( a = start + increment ) + input->dsize[input->ndim-1]; \ \ /* Check for blank values. */ \ if(b==b) do if(*a==b) { hasblank=1; break; } while(++adsize, \ num_increment++, NULL); \ else break; \ } \ } int gal_blank_present(gal_data_t *input, int updateflag) { int hasblank=0; char **str, **strf; size_t increment=0, num_increment=1; gal_data_t *block=gal_tile_block(input); size_t start_end_inc[2]={0,block->size-1}; /* -1: this is INCLUSIVE. */ /* If there is nothing in the array (its size is zero), then return 0 (no blank is present. */ if(input->size==0) return 0; /* From the user's flags, you can tell if the dataset has already been checked for blank values or not. If it has, then just return the checked result. */ if( input->flag & GAL_DATA_FLAG_BLANK_CH ) return input->flag & GAL_DATA_FLAG_HASBLANK; /* Go over the pixels and check: */ switch(block->type) { /* Numeric types */ case GAL_TYPE_UINT8: HAS_BLANK( uint8_t ); break; case GAL_TYPE_INT8: HAS_BLANK( int8_t ); break; case GAL_TYPE_UINT16: HAS_BLANK( uint16_t ); break; case GAL_TYPE_INT16: HAS_BLANK( int16_t ); break; case GAL_TYPE_UINT32: HAS_BLANK( uint32_t ); break; case GAL_TYPE_INT32: HAS_BLANK( int32_t ); break; case GAL_TYPE_UINT64: HAS_BLANK( uint64_t ); break; case GAL_TYPE_INT64: HAS_BLANK( int64_t ); break; case GAL_TYPE_FLOAT32: HAS_BLANK( float ); break; case GAL_TYPE_FLOAT64: HAS_BLANK( double ); break; /* String. */ case GAL_TYPE_STRING: if(input!=block) error(EXIT_FAILURE, 0, "%s: tile mode is currently not supported for " "strings", __func__); strf = (str=input->array) + input->size; do if(!strcmp(*str,GAL_BLANK_STRING)) return 1; while(++strtype); } /* Update the flag if requested. */ if(updateflag) { input->flag |= GAL_DATA_FLAG_BLANK_CH; if(hasblank) input->flag |= GAL_DATA_FLAG_HASBLANK; else input->flag &= ~GAL_DATA_FLAG_HASBLANK; } /* If there was a blank value, then the function would have returned with a value of 1. So if it reaches here, then we can be sure that there was no blank values, hence, return 0. */ return hasblank; } /* Create a dataset of the the same size as the input, but with an uint8_t type that has a value of 1 for data that are blank and 0 for those that aren't. */ #define FLAG_BLANK(IT) { \ IT b, *a=input->array; \ gal_blank_write(&b, input->type); \ if(b==b) /* Blank value can be checked with the equal comparison */ \ do { *o = *a==b; ++a; } while(++oarray, **strf=str+input->size; if( gal_blank_present(input, 0) ) { /* Allocate a non-cleared output array, we are going to parse the input and fill in each element. */ out=gal_data_alloc(NULL, GAL_TYPE_UINT8, input->ndim, input->dsize, input->wcs, 0, input->minmapsize, NULL, "bool", NULL); /* Set the pointers for easy looping. */ of=(o=out->array)+input->size; /* Go over the pixels and set the output values. */ switch(input->type) { /* Numeric types */ case GAL_TYPE_UINT8: FLAG_BLANK( uint8_t ); break; case GAL_TYPE_INT8: FLAG_BLANK( int8_t ); break; case GAL_TYPE_UINT16: FLAG_BLANK( uint16_t ); break; case GAL_TYPE_INT16: FLAG_BLANK( int16_t ); break; case GAL_TYPE_UINT32: FLAG_BLANK( uint32_t ); break; case GAL_TYPE_INT32: FLAG_BLANK( int32_t ); break; case GAL_TYPE_UINT64: FLAG_BLANK( uint64_t ); break; case GAL_TYPE_INT64: FLAG_BLANK( int64_t ); break; case GAL_TYPE_FLOAT32: FLAG_BLANK( float ); break; case GAL_TYPE_FLOAT64: FLAG_BLANK( double ); break; /* String. */ case GAL_TYPE_STRING: do *o++ = !strcmp(*str,GAL_BLANK_STRING); while(++strtype, 1)); /* Bad input. */ default: error(EXIT_FAILURE, 0, "%s: type value (%d) not recognized", __func__, input->type); } } else /* Allocate a CLEAR data structure (all zeros). */ out=gal_data_alloc(NULL, GAL_TYPE_UINT8, input->ndim, input->dsize, input->wcs, 1, input->minmapsize, NULL, "bool", NULL); /* Return */ return out; } /* Remove blank elements from a dataset, convert it to a 1D dataset and adjust the size properly. In practice this function doesn't `realloc' the input array, all it does is to shift the blank eleemnts to the end and adjust the size elements of the `gal_data_t'. */ #define BLANK_REMOVE(IT) { \ IT b, *a=input->array, *af=a+input->size, *o=input->array; \ gal_blank_write(&b, input->type); \ if(b==b) /* Blank value can be be checked with equal. */ \ do if(*a!=b) { ++num; *o++=*a; } while(++ablock && input->ndim!=1 ) error(EXIT_FAILURE, 0, "%s: tiles in datasets with more dimensions than " "1 are not yet supported. Your input has %zu dimensions", __func__, input->ndim); /* If the dataset doesn't have blank values, then just get the size. */ if( gal_blank_present(input, 0) ) { /* Shift all non-blank elements to the start of the array. */ switch(input->type) { case GAL_TYPE_UINT8: BLANK_REMOVE( uint8_t ); break; case GAL_TYPE_INT8: BLANK_REMOVE( int8_t ); break; case GAL_TYPE_UINT16: BLANK_REMOVE( uint16_t ); break; case GAL_TYPE_INT16: BLANK_REMOVE( int16_t ); break; case GAL_TYPE_UINT32: BLANK_REMOVE( uint32_t ); break; case GAL_TYPE_INT32: BLANK_REMOVE( int32_t ); break; case GAL_TYPE_UINT64: BLANK_REMOVE( uint64_t ); break; case GAL_TYPE_INT64: BLANK_REMOVE( int64_t ); break; case GAL_TYPE_FLOAT32: BLANK_REMOVE( float ); break; case GAL_TYPE_FLOAT64: BLANK_REMOVE( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, input->type); } } else num=input->size; /* Adjust the size elements of the dataset. */ input->ndim=1; input->dsize[0]=input->size=num; /* Set the flags to mark that there is no blanks. */ input->flag |= GAL_DATA_FLAG_BLANK_CH; input->flag &= ~GAL_DATA_FLAG_HASBLANK; } /* Print the blank value as a string. For the integer types, we'll use the PRIxNN keywords of `inttypes.h' (which is imported into Gnuastro from Gnulib, so we don't necessarily rely on the host system having it). */ char * gal_blank_as_string(uint8_t type, int width) { char *blank=NULL, *fmt; /* Print the given value. */ switch(type) { case GAL_TYPE_BIT: error(EXIT_FAILURE, 0, "%s: bit types are not implemented yet", __func__); break; case GAL_TYPE_STRING: if(width) asprintf(&blank, "%*s", width, GAL_BLANK_STRING); else asprintf(&blank, "%s", GAL_BLANK_STRING); break; case GAL_TYPE_UINT8: fmt = width ? "%*"PRIu8 : "%"PRIu8; if(width) asprintf(&blank, fmt, width, (uint8_t)GAL_BLANK_UINT8); else asprintf(&blank, fmt, (uint8_t)GAL_BLANK_UINT8); break; case GAL_TYPE_INT8: fmt = width ? "%*"PRId8 : "%"PRId8; if(width) asprintf(&blank, fmt, width, (int8_t)GAL_BLANK_INT8); else asprintf(&blank, fmt, (int8_t)GAL_BLANK_INT8); break; case GAL_TYPE_UINT16: fmt = width ? "%*"PRIu16 : "%"PRIu16; if(width) asprintf(&blank, fmt, width, (uint16_t)GAL_BLANK_UINT16); else asprintf(&blank, fmt, (uint16_t)GAL_BLANK_UINT16); break; case GAL_TYPE_INT16: fmt = width ? "%*"PRId16 : "%"PRId16; if(width) asprintf(&blank, fmt, width, (int16_t)GAL_BLANK_INT16); else asprintf(&blank, fmt, (int16_t)GAL_BLANK_INT16); break; case GAL_TYPE_UINT32: fmt = width ? "%*"PRIu32 : "%"PRIu32; if(width) asprintf(&blank, fmt, width, (uint32_t)GAL_BLANK_UINT32); else asprintf(&blank, fmt, (uint32_t)GAL_BLANK_UINT32); break; case GAL_TYPE_INT32: fmt = width ? "%*"PRId32 : "%"PRId32; if(width) asprintf(&blank, fmt, width, (int32_t)GAL_BLANK_INT32); else asprintf(&blank, fmt, (int32_t)GAL_BLANK_INT32); break; case GAL_TYPE_UINT64: fmt = width ? "%*"PRIu64 : "%"PRIu64; if(width) asprintf(&blank, fmt, width, (uint64_t)GAL_BLANK_UINT64); else asprintf(&blank, fmt, (uint64_t)GAL_BLANK_UINT64); break; case GAL_TYPE_INT64: fmt = width ? "%*"PRId64 : "%"PRId64; if(width) asprintf(&blank, fmt, width, (int64_t)GAL_BLANK_INT64); else asprintf(&blank, fmt, (int64_t)GAL_BLANK_INT64); break; case GAL_TYPE_FLOAT32: if(width) asprintf(&blank, "%*f", width, (float)GAL_BLANK_FLOAT32); else asprintf(&blank, "%f", (float)GAL_BLANK_FLOAT32); break; case GAL_TYPE_FLOAT64: if(width) asprintf(&blank, "%*f", width, (double)GAL_BLANK_FLOAT64); else asprintf(&blank, "%f", (double)GAL_BLANK_FLOAT64); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, type); } return blank; } gnuastro-0.5/lib/binary.c0000644000175000017500000005177113216276304012356 00000000000000/********************************************************************* binary -- Work on binary (0 and 1 valued) datasets. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /*********************************************************************/ /***************** Erosion and dilation ********************/ /*********************************************************************/ static void binary_erode_dilate_2d_4con(gal_data_t *input, int dilate0_erode1) { uint8_t f, b, *pt, *fpt, *byt=input->array; size_t i, j, ind, nr=input->dsize[0], nc=input->dsize[1]; /* Do a sanity check: */ if(dilate0_erode1!=1 && dilate0_erode1!=0) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "fix this problem. The value to `dilate0_erode1' is %u while it " "should be 0 or 1", __func__, PACKAGE_BUGREPORT, dilate0_erode1); /* Set the foreground and background values. */ if(dilate0_erode1==0) {f=1; b=0;} else {f=0; b=1;} /* Check the 4 corners: */ if(byt[0]==b && (byt[1]==f || byt[nc]==f) ) byt[0]=GAL_BINARY_TMP_VALUE; if(byt[nc-1]==b && (byt[nc-2]==f || byt[2*nc-1]==f)) byt[nc-1]=GAL_BINARY_TMP_VALUE; if(byt[(nr-1)*nc]==b && (byt[(nr-2)*nc]==f || byt[(nr-1)*nc+1]==f) ) byt[(nr-1)*nc]=GAL_BINARY_TMP_VALUE; if(byt[nr*nc-1]==b && (byt[nr*nc-2]==f || byt[nr*nc-1-nc]==f) ) byt[nr*nc-1]=GAL_BINARY_TMP_VALUE; /* Check the 4 sides: */ for(j=1;jarray; size_t i, j, ind, nr=input->dsize[0], nc=input->dsize[1]; /* Do a sanity check: */ if(dilate0_erode1!=1 && dilate0_erode1!=0) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can fix " "this problem. The value to dilate0_erode1 is %u while it should " "be 0 or 1", __func__, PACKAGE_BUGREPORT, dilate0_erode1); /* Set the foreground and background values: */ if(dilate0_erode1==0) {f=1; b=0;} else {f=0; b=1;} /* Check the 4 corners: */ if(byt[0]==b && (byt[1]==f || byt[nc]==f || byt[nc+1]==f) ) byt[0]=GAL_BINARY_TMP_VALUE; if(byt[nc-1]==b && (byt[nc-2]==f || byt[2*nc-1]==f || byt[2*nc-2]==f) ) byt[nc-1]=GAL_BINARY_TMP_VALUE; if(byt[(nr-1)*nc]==b && ( byt[(nr-2)*nc]==f || byt[(nr-1)*nc+1]==f || byt[(nr-2)*nc+1]==f) ) byt[(nr-1)*nc]=GAL_BINARY_TMP_VALUE; if(byt[nr*nc-1]==b && ( byt[nr*nc-2]==f || byt[nr*nc-1-nc]==f || byt[nr*nc-2-nc]==f) ) byt[nr*nc-1]=GAL_BINARY_TMP_VALUE; /* Check the 4 sides: */ for(j=1;jndim, input->dsize); /* Currently this only works on blocks. */ if(input->block) error(EXIT_FAILURE, 0, "%s: currently only works on a fully " "allocated block of memory, but the input is a tile (its `block' " "element is not NULL)", __func__); /* Set the dataset to work on. */ binary = ( (inplace && input->type==GAL_TYPE_UINT8) ? input : gal_data_copy_to_new_type(input, GAL_TYPE_UINT8) ); /* Go over every element and do the erosion. */ switch(binary->ndim) { case 2: for(counter=0;counterndim); } /* Clean up and return. */ free(dinc); return binary; } gal_data_t * gal_binary_erode(gal_data_t *input, size_t num, int connectivity, int inplace) { return binary_erode_dilate(input, num, connectivity, inplace, 1); } gal_data_t * gal_binary_dilate(gal_data_t *input, size_t num, int connectivity, int inplace) { return binary_erode_dilate(input, num, connectivity, inplace, 0); } gal_data_t * gal_binary_open(gal_data_t *input, size_t num, int connectivity, int inplace) { gal_data_t *out; /* First do the necessary number of erosions. */ out=gal_binary_erode(input, num, connectivity, inplace); /* If `inplace' was called, then `out' is the same as `input', if it wasn't, then `out' is a newly allocated array. In any case, we should dilate in the same allocated space. */ gal_binary_dilate(input, num, connectivity, 1); /* Return the output dataset. */ return out; } /*********************************************************************/ /***************** Connected components ********************/ /*********************************************************************/ /* Find connected components in an intput dataset. */ size_t gal_binary_connected_components(gal_data_t *binary, gal_data_t **out, int connectivity) { int32_t *l; uint8_t *b, *bf; gal_data_t *lab; size_t p, i, curlab=1; gal_list_sizet_t *Q=NULL; size_t *dinc=gal_dimension_increment(binary->ndim, binary->dsize); /* Two small sanity checks. */ if(binary->type!=GAL_TYPE_UINT8) error(EXIT_FAILURE, 0, "%s: the input data set type must be `uint8'", __func__); if(binary->block) error(EXIT_FAILURE, 0, "%s: currently, the input data structure to " "must not be a tile", __func__); /* Prepare the dataset for the labels. */ if(*out) { /* Use the given dataset. */ lab=*out; /* Make sure the given dataset has the same size as the input. */ if( gal_data_dsize_is_different(binary, lab) ) error(EXIT_FAILURE, 0, "%s: the `binary' and `out' datasets must " "have the same size", __func__); /* Make sure it has a `int32' type. */ if( lab->type!=GAL_TYPE_INT32 ) error(EXIT_FAILURE, 0, "%s: the `out' dataset must have `int32' type" "but the array you have given is `%s' type", __func__, gal_type_name(lab->type, 1)); /* Reset all its values to zero. */ memset(lab->array, 0, lab->size * gal_type_sizeof(lab->type)); } else lab=*out=gal_data_alloc(NULL, GAL_TYPE_INT32, binary->ndim, binary->dsize, binary->wcs, 1, binary->minmapsize, NULL, "labels", NULL); /* Initialize the labels array. If we have blank pixels in the byt array, then give them the blank labeled array. Note that since their value will not be 0, they will also not be labeled. */ l=lab->array; bf=(b=binary->array)+binary->size; /* Library must have no side effect, */ if( gal_blank_present(binary, 0) ) /* So blank flag should not be changed.*/ do *l++ = *b==GAL_BLANK_UINT8 ? GAL_BLANK_INT32 : 0; while(++barray; b=binary->array; for(i=0;isize;++i) /* Check if this pixel is already labeled. */ if( b[i] && l[i]==0 ) { /* This is the first pixel of this connected region that we have got to. */ l[i]=curlab; /* Add this pixel to the queue of pixels to work with. */ gal_list_sizet_add(&Q, i); /* While a pixel remains in the queue, continue labelling and searching for neighbors. */ while(Q!=NULL) { /* Pop an element from the queue. */ p=gal_list_sizet_pop(&Q); /* Go over all its neighbors and add them to the list if they haven't already been labeled. */ GAL_DIMENSION_NEIGHBOR_OP(p, binary->ndim, binary->dsize, connectivity, dinc, { if( b[ nind ] && l[ nind ]==0 ) { l[ nind ] = curlab; gal_list_sizet_add(&Q, nind); } } ); } /* This object has been fully labeled, so increment the current label. */ ++curlab; } /* Clean up and return the total number. */ free(dinc); return curlab-1; } /* Given an adjacency matrix (which should be binary), find the number of connected objects and return an array of new labels for each old label. */ gal_data_t * gal_binary_connected_adjacency_matrix(gal_data_t *adjacency, size_t *numconnected) { gal_data_t *newlabs_d; gal_list_sizet_t *Q=NULL; int32_t *newlabs, curlab=1; uint8_t *adj=adjacency->array; size_t i, j, p, num=adjacency->dsize[0]; /* Some small sanity checks. */ if(adjacency->type != GAL_TYPE_UINT8) error(EXIT_FAILURE, 0, "%s: input must have type `uint8'. However, the " "input dataset has type of `%s'", __func__, gal_type_name(adjacency->type, 1)); if(adjacency->ndim != 2) error(EXIT_FAILURE, 0, "%s: input must be 2-dimensional (a matrix)." "However, the input dataset has %zu dimensions", __func__, adjacency->ndim); if(adjacency->dsize[0] != adjacency->dsize[1]) error(EXIT_FAILURE, 0, "%s: input must be square (same length in both " "dimensions). However, the input dataset has a size of %zu x %zu", __func__, adjacency->dsize[0], adjacency->dsize[1]); /* Allocate (and clear) the output datastructure. */ newlabs_d=gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &num, NULL, 1, adjacency->minmapsize, NULL, NULL, NULL); newlabs=newlabs_d->array; /* Go over the input matrix and apply the same principle as we used to identify connected components in an image: through a queue, find those elements that are connected. */ for(i=1;i new labels ===\n"); for(i=1;indim, __func__, "startcoord"); size_t *dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, input->ndim, __func__, "dsize"); /* Set the size of the padded inverse image and the coordinates of the start. We want the inverse to be padded on the edges of each dimension by 2 pixels, so each dimension should be padded by 4 pixels. */ for(i=0;indim;++i) { startcoord[i]=2; dsize[i]=input->dsize[i]+4; } /* Allocate the inverse dataset and initialize it to 1 (mainly for the edges, the inner region will be set afterwards). PADDING MUST BE INITIALIZED WITH 1: This is done so the connected body of 1 valued pixels (after inversion) gets a label of 1 after labeling the connected components and any hole, will get a value larger than 1. */ inv=gal_data_alloc(NULL, GAL_TYPE_UINT8, input->ndim, dsize, NULL, 0, input->minmapsize, "INVERSE", "binary", NULL); memset(inv->array, 1, inv->size); /* Define a tile to fill the central regions of the inverse. */ startind=gal_dimension_coord_to_index(input->ndim, inv->dsize, startcoord); tile=gal_data_alloc(gal_data_ptr_increment(inv->array, startind, inv->type), inv->type, input->ndim, input->dsize, NULL, 0, 0, NULL, NULL, NULL); *outtile=tile; tile->block=inv; /* Put the input's flags into the inverted array and the tile. */ inv->flag = tile->flag = input->flag; /* Fill the central regions. */ in=input->array; GAL_TILE_PARSE_OPERATE( tile, NULL, 0, 0, {*i = *in==GAL_BLANK_UINT8 ? *in : !*in; ++in;} ); /* Clean up and return. */ free(dsize); free(startcoord); return inv; } /* Fill all the holes in an input unsigned char array. The basic method is this: 1. An inverse image is created: * For every pixel in the input that is 1, the inverse is 0. * The inverse image has two extra pixels on each edge to ensure that all the inv[i]==1 pixels around the image are touching each other and a diagonal object passing through the image does not cause the inv[i]==1 pixels on the edges of the image to get a different label. 2. The 8 connected regions in this inverse image are found. 3. Since we had a 2 pixel padding on the edges of the image, we know for sure that all labeled regions with a label of 1 are actually connected `holes' in the input image. Any pixel with a label larger than 1, is therefore a bounded hole that is not 8-connected to the rest of the holes. */ void gal_binary_fill_holes(gal_data_t *input, int connectivity, size_t maxsize) { uint8_t *in; uint32_t *i, *fi; size_t numholes, *sizes; gal_data_t *inv, *tile, *holelabs=NULL; /* A small sanity check. */ if( input->type != GAL_TYPE_UINT8 ) error(EXIT_FAILURE, 0, "%s: input must have `uint8' type, but its " "input dataset has `%s' type", __func__, gal_type_name(input->type, 1)); /* Make the inverse image. */ inv=binary_make_padded_inverse(input, &tile); /* Label the holes */ numholes=gal_binary_connected_components(inv, &holelabs, connectivity); /* Any pixel with a label larger than 1 is a hole in the input image and we should invert the respective pixel. To do it, we'll use the tile that was defined before, just change its block and array.*/ in=input->array; tile->array=gal_tile_block_relative_to_other(tile, holelabs); tile->block=holelabs; /* has to be after correcting `tile->array'. */ /* If the user wants to only fill holes to a certain size, then remove those with a larger size. */ if(maxsize<-1) { /* Allocate space to keep the size of each hole: */ sizes=gal_data_calloc_array(GAL_TYPE_SIZE_T, numholes+1, __func__, "sizes"); fi=(i=holelabs->array)+holelabs->size; do ++sizes[*i]; while(++iarray)+holelabs->size; do if(*i!=GAL_BLANK_INT32) *i = sizes[*i]>maxsize ? 1 : *i; while(++i1 && *i!=GAL_BLANK_INT32 ? 1 : *in; ++in; }); /* Clean up and return. */ tile->array=NULL; gal_data_free(inv); gal_data_free(tile); gal_data_free(holelabs); } gnuastro-0.5/lib/arithmetic-plus.c0000644000175000017500000000361113215601241014161 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_plus(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), + ); } gnuastro-0.5/lib/arithmetic-or.c0000644000175000017500000000345113215601241013620 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_or(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, || ); } gnuastro-0.5/lib/arithmetic-ne.c0000644000175000017500000000345113215601241013602 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_ne(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, != ); } gnuastro-0.5/lib/arithmetic-multiply.c0000644000175000017500000000361513215601241015061 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_multiply(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), * ); } gnuastro-0.5/lib/arithmetic-modulo.c0000644000175000017500000000414013215601241014473 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* `BINARY_SET_LT_INT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_modulo(gal_data_t *l, gal_data_t *r, gal_data_t *o) { /* A small sanity check. */ if( l->type==GAL_TYPE_FLOAT32 || l->type==GAL_TYPE_FLOAT64 || r->type==GAL_TYPE_FLOAT32 || r->type==GAL_TYPE_FLOAT64 ) error(EXIT_FAILURE, 0, "%s: the modulo operator can only work on " "integer type operands", __func__); /* Do the operation. */ BINARY_SET_LT_INT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), % ); } gnuastro-0.5/lib/arithmetic-minus.c0000644000175000017500000000361213215601241014332 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_minus(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), - ); } gnuastro-0.5/lib/arithmetic-lt.c0000644000175000017500000000345013215601241013616 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_lt(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, < ); } gnuastro-0.5/lib/arithmetic-le.c0000644000175000017500000000345113215601241013600 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_le(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, <= ); } gnuastro-0.5/lib/arithmetic-gt.c0000644000175000017500000000345013215601241013611 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_gt(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, > ); } gnuastro-0.5/lib/arithmetic-ge.c0000644000175000017500000000345113215601241013573 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_ge(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, >= ); } gnuastro-0.5/lib/arithmetic-eq.c0000644000175000017500000000345113215601241013605 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_eq(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, == ); } gnuastro-0.5/lib/arithmetic-divide.c0000644000175000017500000000361313215601241014444 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_divide(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), / ); } gnuastro-0.5/lib/arithmetic-bitxor.c0000644000175000017500000000414013215601241014503 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* `BINARY_SET_LT_INT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_bitxor(gal_data_t *l, gal_data_t *r, gal_data_t *o) { /* A small sanity check. */ if( l->type==GAL_TYPE_FLOAT32 || l->type==GAL_TYPE_FLOAT64 || r->type==GAL_TYPE_FLOAT32 || r->type==GAL_TYPE_FLOAT64 ) error(EXIT_FAILURE, 0, "%s: the bitxor operator can only work on " "integer type operands", __func__); /* Do the operation. */ BINARY_SET_LT_INT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), ^ ); } gnuastro-0.5/lib/arithmetic-bitrsh.c0000644000175000017500000000414113215601241014470 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* `BINARY_SET_LT_INT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_bitrsh(gal_data_t *l, gal_data_t *r, gal_data_t *o) { /* A small sanity check. */ if( l->type==GAL_TYPE_FLOAT32 || l->type==GAL_TYPE_FLOAT64 || r->type==GAL_TYPE_FLOAT32 || r->type==GAL_TYPE_FLOAT64 ) error(EXIT_FAILURE, 0, "%s: the bitrsh operator can only work on " "integer type operands", __func__); /* Do the operation. */ BINARY_SET_LT_INT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), >> ); } gnuastro-0.5/lib/arithmetic-bitor.c0000644000175000017500000000413613215601241014320 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* `BINARY_SET_LT_INT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_bitor(gal_data_t *l, gal_data_t *r, gal_data_t *o) { /* A small sanity check. */ if( l->type==GAL_TYPE_FLOAT32 || l->type==GAL_TYPE_FLOAT64 || r->type==GAL_TYPE_FLOAT32 || r->type==GAL_TYPE_FLOAT64 ) error(EXIT_FAILURE, 0, "%s: the bitor operator can only work on " "integer type operands", __func__); /* Do the operation. */ BINARY_SET_LT_INT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), | ); } gnuastro-0.5/lib/arithmetic-bitlsh.c0000644000175000017500000000414113215601241014462 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* `BINARY_SET_LT_INT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_bitlsh(gal_data_t *l, gal_data_t *r, gal_data_t *o) { /* A small sanity check. */ if( l->type==GAL_TYPE_FLOAT32 || l->type==GAL_TYPE_FLOAT64 || r->type==GAL_TYPE_FLOAT32 || r->type==GAL_TYPE_FLOAT64 ) error(EXIT_FAILURE, 0, "%s: the bitlsh operator can only work on " "integer type operands", __func__); /* Do the operation. */ BINARY_SET_LT_INT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), << ); } gnuastro-0.5/lib/arithmetic-bitand.c0000644000175000017500000000414013215601241014435 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include /* `BINARY_SET_LT_INT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_bitand(gal_data_t *l, gal_data_t *r, gal_data_t *o) { /* A small sanity check. */ if( l->type==GAL_TYPE_FLOAT32 || l->type==GAL_TYPE_FLOAT64 || r->type==GAL_TYPE_FLOAT32 || r->type==GAL_TYPE_FLOAT64 ) error(EXIT_FAILURE, 0, "%s: the bitand operator can only work on " "integer type operands", __func__); /* Do the operation. */ BINARY_SET_LT_INT( ( o->type==l->type ? ARITHMETIC_BINARY_OUT_TYPE_LEFT : ARITHMETIC_BINARY_OUT_TYPE_RIGHT ), & ); } gnuastro-0.5/lib/arithmetic-and.c0000644000175000017500000000345213215601241013743 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include /* `BINARY_SET_LT' is defined in `arithmetic-binary.h'. As you see there, this is a deep macro (calls other macros) to deal with different types. This allows efficiency in processing (after compilation), but compilation will be very slow. Therefore, for each operator we have defined a separate `.c' file so they are built separately and when built in parallel can be much faster than having them all in a single file. */ void arithmetic_and(gal_data_t *l, gal_data_t *r, gal_data_t *o) { int checkblank=gal_arithmetic_binary_checkblank(l, r); BINARY_SET_LT( ARITHMETIC_BINARY_OUT_TYPE_UINT8, && ); } gnuastro-0.5/lib/arithmetic.c0000644000175000017500000017212113215601241013203 00000000000000/********************************************************************* Arithmetic operations on data structures This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #include #include #include #include #include #include #include #include #include #include #include /* Headers for each binary operator. Since they heavily involve macros, their compilation can be very large if they are in a single function and file. So there is a separate C source and header file for each of these functions.*/ #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include /***********************************************************************/ /*************** Internal checks **************/ /***********************************************************************/ /* Some functions are only for a floating point operand, so if the input isn't floating point, inform the user to change the type explicitly, doing it implicitly/internally puts too much responsability on the program. */ static void arithmetic_check_float_input(gal_data_t *in, int operator, char *numstr) { switch(in->type) { case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: break; default: error(EXIT_FAILURE, 0, "the %s operator can only accept single or " "double precision floating point numbers as its operand. The " "%s operand has type %s. You can use the `float' or `double' " "operators before this operator to explicitly convert to the " "desired precision floating point type. If the operand was " "originally a typed number (string of characters), add an `f' " "after it so it is directly read into the proper precision " "floating point number (based on the number of non-zero " "decimals it has)", gal_arithmetic_operator_string(operator), numstr, gal_type_name(in->type, 1)); } } /***********************************************************************/ /*************** Unary functions/operators **************/ /***********************************************************************/ /* Change input data structure type. */ static gal_data_t * arithmetic_change_type(gal_data_t *data, int operator, int flags) { int type=-1; gal_data_t *out; /* Set the output type. */ switch(operator) { case GAL_ARITHMETIC_OP_TO_UINT8: type=GAL_TYPE_UINT8; break; case GAL_ARITHMETIC_OP_TO_INT8: type=GAL_TYPE_INT8; break; case GAL_ARITHMETIC_OP_TO_UINT16: type=GAL_TYPE_UINT16; break; case GAL_ARITHMETIC_OP_TO_INT16: type=GAL_TYPE_INT16; break; case GAL_ARITHMETIC_OP_TO_UINT32: type=GAL_TYPE_UINT32; break; case GAL_ARITHMETIC_OP_TO_INT32: type=GAL_TYPE_INT32; break; case GAL_ARITHMETIC_OP_TO_UINT64: type=GAL_TYPE_UINT64; break; case GAL_ARITHMETIC_OP_TO_INT64: type=GAL_TYPE_INT64; break; case GAL_ARITHMETIC_OP_TO_FLOAT32: type=GAL_TYPE_FLOAT32; break; case GAL_ARITHMETIC_OP_TO_FLOAT64: type=GAL_TYPE_FLOAT64; break; default: error(EXIT_FAILURE, 0, "%s: operator value of %d not recognized", __func__, operator); } /* Copy to the new type. */ out=gal_data_copy_to_new_type(data, type); /* Delete the input structure if the user asked for it. */ if(flags & GAL_ARITHMETIC_FREE) gal_data_free(data); /* Return */ return out; } /* Return an array of value 1 for any zero valued element and zero for any non-zero valued element. */ #define TYPE_CASE_FOR_NOT(CTYPE) { \ CTYPE *a=data->array, *af=a+data->size; \ do *o++ = !(*a); while(++andim, data->dsize, data->wcs, 0, data->minmapsize, data->name, data->unit, data->comment); o=out->array; /* Go over the pixels and set the output values. */ switch(data->type) { case GAL_TYPE_UINT8: TYPE_CASE_FOR_NOT(uint8_t); break; case GAL_TYPE_INT8: TYPE_CASE_FOR_NOT(int8_t); break; case GAL_TYPE_UINT16: TYPE_CASE_FOR_NOT(uint16_t); break; case GAL_TYPE_INT16: TYPE_CASE_FOR_NOT(int16_t); break; case GAL_TYPE_UINT32: TYPE_CASE_FOR_NOT(uint32_t); break; case GAL_TYPE_INT32: TYPE_CASE_FOR_NOT(int32_t); break; case GAL_TYPE_UINT64: TYPE_CASE_FOR_NOT(uint64_t); break; case GAL_TYPE_INT64: TYPE_CASE_FOR_NOT(int64_t); break; case GAL_TYPE_FLOAT32: TYPE_CASE_FOR_NOT(float); break; case GAL_TYPE_FLOAT64: TYPE_CASE_FOR_NOT(double); break; case GAL_TYPE_BIT: error(EXIT_FAILURE, 0, "%s: bit datatypes are not yet supported, " "please get in touch with us to implement it.", __func__); default: error(EXIT_FAILURE, 0, "%s: type value (%d) not recognized", __func__, data->type); } /* Delete the input structure if the user asked for it. */ if(flags & GAL_ARITHMETIC_FREE) gal_data_free(data); /* Return */ return out; } /* Bitwise not operator. */ static gal_data_t * arithmetic_bitwise_not(int flags, gal_data_t *in) { gal_data_t *o; uint8_t *iu8 = in->array, *iu8f = iu8 + in->size, *ou8; int8_t *ii8 = in->array, *ii8f = ii8 + in->size, *oi8; uint16_t *iu16 = in->array, *iu16f = iu16 + in->size, *ou16; int16_t *ii16 = in->array, *ii16f = ii16 + in->size, *oi16; uint32_t *iu32 = in->array, *iu32f = iu32 + in->size, *ou32; int32_t *ii32 = in->array, *ii32f = ii32 + in->size, *oi32; uint64_t *iu64 = in->array, *iu64f = iu64 + in->size, *ou64; int64_t *ii64 = in->array, *ii64f = ii64 + in->size, *oi64; /* Check the type */ switch(in->type) { case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: error(EXIT_FAILURE, 0, "%s: bitwise not (one's complement) " "operator can only work on integer types", __func__); } /* If we want inplace output, set the output pointer to the input pointer, for every pixel, the operation will be independent. */ if(flags & GAL_ARITHMETIC_INPLACE) o = in; else o = gal_data_alloc(NULL, in->type, in->ndim, in->dsize, in->wcs, 0, in->minmapsize, NULL, NULL, NULL); /* Start setting the types. */ switch(in->type) { case GAL_TYPE_UINT8: ou8=o->array; do *ou8++ = ~(*iu8++); while(iu8array; do *oi8++ = ~(*ii8++); while(ii8array; do *ou16++ = ~(*iu16++); while(iu16array; do *oi16++ = ~(*ii16++); while(ii16array; do *ou32++ = ~(*iu32++); while(iu32array; do *oi32++ = ~(*ii32++); while(ii32array; do *ou64++ = ~(*iu64++); while(iu64array; do *oi64++ = ~(*ii64++); while(ii64type); } /* Clean up (if necessary). */ if( (flags & GAL_ARITHMETIC_FREE) && o!=in) gal_data_free(in); /* Return */ return o; } /* We don't want to use the standard function for unary functions in the case of the absolute operator. This is because there are multiple versions of this function in the C library for different types, which can greatly improve speed. */ #define ARITHMETIC_ABS_SGN(CTYPE, FUNC) { \ CTYPE *o=out->array, *a=in->array, *af=a+in->size; \ do *o++ = FUNC(*a); while(++atype, in->ndim, in->dsize, in->wcs, 0, in->minmapsize, in->name, in->unit, in->comment); /* Put the absolute value depending on the type. */ switch(in->type) { /* Unsigned types are already positive, so if the input is not to be freed (the output must be a separate array), just copy the whole array. */ case GAL_TYPE_UINT8: case GAL_TYPE_UINT16: case GAL_TYPE_UINT32: case GAL_TYPE_UINT64: if(out!=in) gal_data_copy_to_allocated(in, out); break; /* For the signed types, we actually have to go over the data and calculate the absolute value. There are unique functions for different types, so we will be using them.*/ case GAL_TYPE_INT8: ARITHMETIC_ABS_SGN( int8_t, abs ); break; case GAL_TYPE_INT16: ARITHMETIC_ABS_SGN( int16_t, abs ); break; case GAL_TYPE_INT32: ARITHMETIC_ABS_SGN( int32_t, labs ); break; case GAL_TYPE_INT64: ARITHMETIC_ABS_SGN( int64_t, llabs ); break; case GAL_TYPE_FLOAT32: ARITHMETIC_ABS_SGN( float, fabsf ); break; case GAL_TYPE_FLOAT64: ARITHMETIC_ABS_SGN( double, fabs ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, in->type); } /* Clean up and return */ if( (flags & GAL_ARITHMETIC_FREE) && out!=in) gal_data_free(in); return out; } #define UNIFUNC_RUN_FUNCTION_ON_ELEMENT(IT, OP){ \ IT *ia=in->array, *oa=o->array, *iaf=ia + in->size; \ do *oa++ = OP(*ia++); while(iatype) \ { \ case GAL_TYPE_UINT8: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(uint8_t, OP) \ break; \ case GAL_TYPE_INT8: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(int8_t, OP) \ break; \ case GAL_TYPE_UINT16: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(uint16_t, OP) \ break; \ case GAL_TYPE_INT16: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(int16_t, OP) \ break; \ case GAL_TYPE_UINT32: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(uint32_t, OP) \ break; \ case GAL_TYPE_INT32: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(int32_t, OP) \ break; \ case GAL_TYPE_UINT64: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(uint64_t, OP) \ break; \ case GAL_TYPE_INT64: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(int64_t, OP) \ break; \ case GAL_TYPE_FLOAT32: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(float, OP) \ break; \ case GAL_TYPE_FLOAT64: \ UNIFUNC_RUN_FUNCTION_ON_ELEMENT(double, OP) \ break; \ default: \ error(EXIT_FAILURE, 0, "%s: type code %d not recognized", \ "UNIARY_FUNCTION_ON_ELEMENT", in->type); \ } static gal_data_t * arithmetic_unary_function(int operator, int flags, gal_data_t *in) { gal_data_t *o; /* If we want inplace output, set the output pointer to the input pointer, for every pixel, the operation will be independent. */ if(flags & GAL_ARITHMETIC_INPLACE) o = in; else o = gal_data_alloc(NULL, in->type, in->ndim, in->dsize, in->wcs, 0, in->minmapsize, NULL, NULL, NULL); /* Start setting the operator and operands. */ switch(operator) { case GAL_ARITHMETIC_OP_SQRT: UNIARY_FUNCTION_ON_ELEMENT( sqrt ); break; case GAL_ARITHMETIC_OP_LOG: UNIARY_FUNCTION_ON_ELEMENT( log ); break; case GAL_ARITHMETIC_OP_LOG10: UNIARY_FUNCTION_ON_ELEMENT( log10 ); break; default: error(EXIT_FAILURE, 0, "%s: operator code %d not recognized", __func__, operator); } /* Clean up. Note that if the input arrays can be freed, and any of right or left arrays needed conversion, `UNIFUNC_CONVERT_TO_COMPILED_TYPE' has already freed the input arrays, and we only have `r' and `l' allocated in any case. Alternatively, when the inputs shouldn't be freed, the only allocated spaces are the `r' and `l' arrays if their types weren't compiled for binary operations, we can tell this from the pointers: if they are different from the original pointers, they were allocated. */ if( (flags & GAL_ARITHMETIC_FREE) && o!=in) gal_data_free(in); /* Return */ return o; } /* Call functions in the `gnuastro/statistics' library. */ static gal_data_t * arithmetic_from_statistics(int operator, int flags, gal_data_t *input) { gal_data_t *out=NULL; int ip=(flags & GAL_ARITHMETIC_INPLACE) || (flags & GAL_ARITHMETIC_FREE); switch(operator) { case GAL_ARITHMETIC_OP_MINVAL: out=gal_statistics_minimum(input); break; case GAL_ARITHMETIC_OP_MAXVAL: out=gal_statistics_maximum(input); break; case GAL_ARITHMETIC_OP_NUMVAL: out=gal_statistics_number(input); break; case GAL_ARITHMETIC_OP_SUMVAL: out=gal_statistics_sum(input); break; case GAL_ARITHMETIC_OP_MEANVAL: out=gal_statistics_mean(input); break; case GAL_ARITHMETIC_OP_STDVAL: out=gal_statistics_std(input); break; case GAL_ARITHMETIC_OP_MEDIANVAL: out=gal_statistics_median(input, ip); break; default: error(EXIT_FAILURE, 0, "%s: operator code %d not recognized", __func__, operator); } /* If the input is to be freed, then do so and return the output. */ if( flags & GAL_ARITHMETIC_FREE ) gal_data_free(input); return out; } /***********************************************************************/ /*************** Where **************/ /***********************************************************************/ /* When the `iftrue' dataset only has one element and the element is blank, then it will be replaced with the blank value of the type of the output data. */ #define DO_WHERE_OPERATION(ITT, OT) { \ ITT *it=iftrue->array; \ OT b, *o=out->array, *of=o+out->size; \ if(iftrue->size==1) \ { \ if( gal_blank_present(iftrue, 0) ) \ { \ gal_blank_write(&b, out->type); \ do { *o = *c++ ? b : *o; } while(++otype) \ { \ case GAL_TYPE_UINT8: DO_WHERE_OPERATION( uint8_t, OT); break; \ case GAL_TYPE_INT8: DO_WHERE_OPERATION( int8_t, OT); break; \ case GAL_TYPE_UINT16: DO_WHERE_OPERATION( uint16_t, OT); break; \ case GAL_TYPE_INT16: DO_WHERE_OPERATION( int16_t, OT); break; \ case GAL_TYPE_UINT32: DO_WHERE_OPERATION( uint32_t, OT); break; \ case GAL_TYPE_INT32: DO_WHERE_OPERATION( int32_t, OT); break; \ case GAL_TYPE_UINT64: DO_WHERE_OPERATION( uint64_t, OT); break; \ case GAL_TYPE_INT64: DO_WHERE_OPERATION( int64_t, OT); break; \ case GAL_TYPE_FLOAT32: DO_WHERE_OPERATION( float, OT); break; \ case GAL_TYPE_FLOAT64: DO_WHERE_OPERATION( double, OT); break; \ default: \ error(EXIT_FAILURE, 0, "%s: type code %d not recognized for the " \ "`iftrue' dataset", "WHERE_OUT_SET", iftrue->type); \ } static void arithmetic_where(int flags, gal_data_t *out, gal_data_t *cond, gal_data_t *iftrue) { unsigned char *c=cond->array; /* The condition operator has to be unsigned char. */ if(cond->type!=GAL_TYPE_UINT8) error(EXIT_FAILURE, 0, "%s: the condition operand must be an " "`uint8' type, but the given condition operand has a " "`%s' type", __func__, gal_type_name(cond->type, 1)); /* The dimension and sizes of the out and condition data sets must be the same. */ if(gal_data_dsize_is_different(out, cond)) error(EXIT_FAILURE, 0, "%s: the output and condition data sets of the " "must be the same size", __func__); /* Do the operation. */ switch(out->type) { case GAL_TYPE_UINT8: WHERE_OUT_SET( uint8_t ); break; case GAL_TYPE_INT8: WHERE_OUT_SET( int8_t ); break; case GAL_TYPE_UINT16: WHERE_OUT_SET( uint16_t ); break; case GAL_TYPE_INT16: WHERE_OUT_SET( int16_t ); break; case GAL_TYPE_UINT32: WHERE_OUT_SET( uint32_t ); break; case GAL_TYPE_INT32: WHERE_OUT_SET( int32_t ); break; case GAL_TYPE_UINT64: WHERE_OUT_SET( uint64_t ); break; case GAL_TYPE_INT64: WHERE_OUT_SET( int64_t ); break; case GAL_TYPE_FLOAT32: WHERE_OUT_SET( float ); break; case GAL_TYPE_FLOAT64: WHERE_OUT_SET( double ); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized for the `out'", __func__, out->type); } /* Clean up if necessary. */ if(flags & GAL_ARITHMETIC_FREE) { gal_data_free(cond); gal_data_free(iftrue); } } /***********************************************************************/ /*************** Multiple operand operators **************/ /***********************************************************************/ #define MULTIOPERAND_MIN(TYPE) { \ TYPE p, max; \ size_t n, j=0; \ gal_type_max(list->type, &max); \ do /* Loop over each pixel */ \ { \ n=0; \ p=max; \ for(i=0;itype, &min); \ do /* Loop over each pixel */ \ { \ n=0; \ p=min; \ for(i=0;i p ? a[i][j] : p; ++n; } \ } \ else { p = a[i][j] > p ? a[i][j] : p; ++n; } \ } \ *o++ = n ? p : b; /* No usable elements: set to blank. */ \ ++j; \ } \ while(otype, dnum, __func__, "pixs"); \ \ /* Loop over each pixel */ \ do \ { \ /* Initialize. */ \ n=0; \ \ /* Loop over each array. */ \ for(i=0;iarray, *of=o+out->size; \ size_t i=0; /* Different from the `i' in the main function. */ \ \ /* Allocate space to keep the pointers to the arrays of each. */ \ /* Input data structure. The operators will increment these */ \ /* pointers while parsing them. */ \ errno=0; \ a=malloc(dnum*sizeof *a); \ if(a==NULL) \ error(EXIT_FAILURE, 0, "%s: %zu bytes for `a'", \ "MULTIOPERAND_TYPE_SET", dnum*sizeof *a); \ \ /* Fill in the array pointers and the blank value for this type. */ \ gal_blank_write(&b, list->type); \ for(tmp=list;tmp!=NULL;tmp=tmp->next) \ a[i++]=tmp->array; \ \ /* Do the operation. */ \ switch(operator) \ { \ case GAL_ARITHMETIC_OP_MIN: \ MULTIOPERAND_MIN(TYPE); \ break; \ \ case GAL_ARITHMETIC_OP_MAX: \ MULTIOPERAND_MAX(TYPE); \ break; \ \ case GAL_ARITHMETIC_OP_NUM: \ MULTIOPERAND_NUM; \ break; \ \ case GAL_ARITHMETIC_OP_SUM: \ MULTIOPERAND_SUM; \ break; \ \ case GAL_ARITHMETIC_OP_MEAN: \ MULTIOPERAND_MEAN; \ break; \ \ case GAL_ARITHMETIC_OP_STD: \ MULTIOPERAND_STD; \ break; \ \ case GAL_ARITHMETIC_OP_MEDIAN: \ MULTIOPERAND_MEDIAN(TYPE, QSORT_F); \ break; \ \ default: \ error(EXIT_FAILURE, 0, "%s: operator code %d not recognized", \ "MULTIOPERAND_TYPE_SET", operator); \ } \ \ /* Clean up. */ \ free(a); \ } /* The single operator in this function is assumed to be a linked list. The number of operators is determined from the fact that the last node in the linked list must have a NULL pointer as its `next' element.*/ static gal_data_t * arithmetic_multioperand(int operator, int flags, gal_data_t *list) { uint8_t *hasblank; size_t i=0, dnum=1; gal_data_t *out, *tmp, *ttmp; /* For generality, `list' can be a NULL pointer, in that case, this function will return a NULL pointer and avoid further processing. */ if(list==NULL) return NULL; /* Do a simple sanity check, comparing the operand on top of the list to the rest of the operands within the list. */ for(tmp=list->next;tmp!=NULL;tmp=tmp->next) { /* Increment the number of structures. */ ++dnum; /* Check the types. */ if(tmp->type!=list->type) error(EXIT_FAILURE, 0, "%s: the types of all operands to the %s " "operator must be same", __func__, gal_arithmetic_operator_string(operator)); /* Check the sizes. */ if( gal_data_dsize_is_different(list, tmp) ) error(EXIT_FAILURE, 0, "%s: the sizes of all operands to the %s " "operator must be same", __func__, gal_arithmetic_operator_string(operator)); } /* Set the output data structure. */ if(flags & GAL_ARITHMETIC_INPLACE) out = list; /* The top element in the list. */ else out = gal_data_alloc(NULL, list->type, list->ndim, list->dsize, list->wcs, 0, list->minmapsize, NULL, NULL, NULL); /* hasblank is used to see if a blank value should be checked for each list element or not. */ hasblank=gal_data_malloc_array(GAL_TYPE_UINT8, dnum, __func__, "hasblank"); for(tmp=list;tmp!=NULL;tmp=tmp->next) hasblank[i++]=gal_blank_present(tmp, 0); /* Start the operation. */ switch(list->type) { case GAL_TYPE_UINT8: MULTIOPERAND_TYPE_SET(uint8_t, gal_qsort_uint8_increasing); break; case GAL_TYPE_INT8: MULTIOPERAND_TYPE_SET(int8_t, gal_qsort_int8_increasing); break; case GAL_TYPE_UINT16: MULTIOPERAND_TYPE_SET(uint16_t, gal_qsort_uint16_increasing); break; case GAL_TYPE_INT16: MULTIOPERAND_TYPE_SET(int16_t, gal_qsort_int16_increasing); break; case GAL_TYPE_UINT32: MULTIOPERAND_TYPE_SET(uint32_t, gal_qsort_uint32_increasing); break; case GAL_TYPE_INT32: MULTIOPERAND_TYPE_SET(int32_t, gal_qsort_int32_increasing); break; case GAL_TYPE_UINT64: MULTIOPERAND_TYPE_SET(uint64_t, gal_qsort_uint64_increasing); break; case GAL_TYPE_INT64: MULTIOPERAND_TYPE_SET(int64_t, gal_qsort_int64_increasing); break; case GAL_TYPE_FLOAT32: MULTIOPERAND_TYPE_SET(float, gal_qsort_float32_increasing); break; case GAL_TYPE_FLOAT64: MULTIOPERAND_TYPE_SET(double, gal_qsort_float64_increasing); break; default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, list->type); } /* Clean up and return. Note that the operation might have been done in place. In that case, the top most list element was used. So we need to check before freeing each data structure. */ if(flags & GAL_ARITHMETIC_FREE) { tmp=list; while(tmp!=NULL) { ttmp=tmp->next; if(tmp!=out) gal_data_free(tmp); tmp=ttmp; } } free(hasblank); return out; } /**********************************************************************/ /**************** Binary operators *****************/ /**********************************************************************/ /* See if we should check for blanks. When both types are floats, blanks don't need to be checked (the floating point standard will do the job for us). It is also not necessary to check blanks in bitwise operators, but bitwise operators have their own macro (`BINARY_OP_INCR_OT_RT_LT_SET') which doesn' use `checkblanks'.*/ int gal_arithmetic_binary_checkblank(gal_data_t *l, gal_data_t *r) { return ((((l->type!=GAL_TYPE_FLOAT32 && l->type!=GAL_TYPE_FLOAT64) || (r->type!=GAL_TYPE_FLOAT32 && r->type!=GAL_TYPE_FLOAT64)) && (gal_blank_present(l, 1) || gal_blank_present(r, 1))) ? 1 : 0 ); } static int arithmetic_binary_out_type(int operator, gal_data_t *l, gal_data_t *r) { switch(operator) { case GAL_ARITHMETIC_OP_PLUS: case GAL_ARITHMETIC_OP_MINUS: case GAL_ARITHMETIC_OP_MULTIPLY: case GAL_ARITHMETIC_OP_DIVIDE: return gal_type_out(l->type, r->type); default: return GAL_TYPE_UINT8; } return -1; } static gal_data_t * arithmetic_binary(int operator, int flags, gal_data_t *l, gal_data_t *r) { /* Read the variable arguments. `lo' and `ro' keep the original data, in case their type isn't built (based on configure options are configure time). */ int32_t otype; gal_data_t *o=NULL; size_t out_size, minmapsize; /* Simple sanity check on the input sizes */ if( !( (flags & GAL_ARITHMETIC_NUMOK) && (l->size==1 || r->size==1)) && gal_data_dsize_is_different(l, r) ) error(EXIT_FAILURE, 0, "%s: the non-number inputs to %s don't have the " "same dimension/size", __func__, gal_arithmetic_operator_string(operator)); /* Set the output type. For the comparison operators, the output type is either 0 or 1, so we will set the output type to `unsigned char' for efficient memory and CPU usage. Since the number of operators without a fixed output type (like the conditionals) is less, by `default' we will set the output type to `unsigned char', and if any of the other operatrs are given, it will be chosen based on the input types.*/ otype=arithmetic_binary_out_type(operator, l, r); /* Set the output sizes. */ minmapsize = ( l->minmapsize < r->minmapsize ? l->minmapsize : r->minmapsize ); out_size = l->size > r->size ? l->size : r->size; /* If we want inplace output, set the output pointer to one input. Note that the output type can be different from both inputs. */ if(flags & GAL_ARITHMETIC_INPLACE) { if (l->type==otype && out_size==l->size) o = l; else if(r->type==otype && out_size==r->size) o = r; } /* If the output pointer was not set above for any of the possible reasons, allocate it. For `mmapsize', note that since its `size_t', it will always be positive. The `-1' that is recommended to give when you want the value in RAM is actually the largest possible memory location. So we just have to choose the smaller minmapsize of the two to decide if the output array should be in RAM or not. */ if(o==NULL) o = gal_data_alloc(NULL, otype, l->size>1 ? l->ndim : r->ndim, l->size>1 ? l->dsize : r->dsize, l->size>1 ? l->wcs : r->wcs, 0, minmapsize, NULL, NULL, NULL ); /* Call the proper function for the operator. Since they heavily involve macros, their compilation can be very large if they are in a single function and file. So there is a separate C source and header file for each of these functions. */ switch(operator) { case GAL_ARITHMETIC_OP_PLUS: arithmetic_plus(l, r, o); break; case GAL_ARITHMETIC_OP_MINUS: arithmetic_minus(l, r, o); break; case GAL_ARITHMETIC_OP_MULTIPLY: arithmetic_multiply(l, r, o); break; case GAL_ARITHMETIC_OP_DIVIDE: arithmetic_divide(l, r, o); break; case GAL_ARITHMETIC_OP_LT: arithmetic_lt(l, r, o); break; case GAL_ARITHMETIC_OP_LE: arithmetic_le(l, r, o); break; case GAL_ARITHMETIC_OP_GT: arithmetic_gt(l, r, o); break; case GAL_ARITHMETIC_OP_GE: arithmetic_ge(l, r, o); break; case GAL_ARITHMETIC_OP_EQ: arithmetic_eq(l, r, o); break; case GAL_ARITHMETIC_OP_NE: arithmetic_ne(l, r, o); break; case GAL_ARITHMETIC_OP_AND: arithmetic_and(l, r, o); break; case GAL_ARITHMETIC_OP_OR: arithmetic_or(l, r, o); break; case GAL_ARITHMETIC_OP_BITAND: arithmetic_bitand(l, r, o); break; case GAL_ARITHMETIC_OP_BITOR: arithmetic_bitor(l, r, o); break; case GAL_ARITHMETIC_OP_BITXOR: arithmetic_bitxor(l, r, o); break; case GAL_ARITHMETIC_OP_BITLSH: arithmetic_bitlsh(l, r, o); break; case GAL_ARITHMETIC_OP_BITRSH: arithmetic_bitrsh(l, r, o); break; case GAL_ARITHMETIC_OP_MODULO: arithmetic_modulo(l, r, o); break; default: error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to address " "the problem. %d is not a valid operator code", __func__, PACKAGE_BUGREPORT, operator); } /* Clean up if necessary. Note that if the operation was requested to be in place, then the output might be one of the inputs. */ if(flags & GAL_ARITHMETIC_FREE) { if (o==l) gal_data_free(r); else if(o==r) gal_data_free(l); else { gal_data_free(l); gal_data_free(r); } } /* Return */ return o; } #define BINFUNC_RUN_FUNCTION(OT, RT, LT, OP){ \ LT *la=l->array; \ RT *ra=r->array; \ OT *oa=o->array, *of=oa + o->size; \ if(l->size==r->size) do *oa = OP(*la++, *ra++); while(++oasize==1) do *oa = OP(*la, *ra++); while(++oatype) \ { \ case GAL_TYPE_FLOAT32: \ BINFUNC_RUN_FUNCTION(float, RT, LT, OP); \ break; \ case GAL_TYPE_FLOAT64: \ BINFUNC_RUN_FUNCTION(double, RT, LT, OP); \ break; \ default: \ error(EXIT_FAILURE, 0, "%s: type %d not recognized for o->type ", \ "BINFUNC_F_OPERATOR_LEFT_RIGHT_SET", o->type); \ } #define BINFUNC_F_OPERATOR_LEFT_SET(LT, OP) \ switch(r->type) \ { \ case GAL_TYPE_FLOAT32: \ BINFUNC_F_OPERATOR_LEFT_RIGHT_SET(float, LT, OP); \ break; \ case GAL_TYPE_FLOAT64: \ BINFUNC_F_OPERATOR_LEFT_RIGHT_SET(double, LT, OP); \ break; \ default: \ error(EXIT_FAILURE, 0, "%s: type %d not recognized for r->type", \ "BINFUNC_F_OPERATOR_LEFT_SET", r->type); \ } #define BINFUNC_F_OPERATOR_SET(OP) \ switch(l->type) \ { \ case GAL_TYPE_FLOAT32: \ BINFUNC_F_OPERATOR_LEFT_SET(float, OP); \ break; \ case GAL_TYPE_FLOAT64: \ BINFUNC_F_OPERATOR_LEFT_SET(double, OP); \ break; \ default: \ error(EXIT_FAILURE, 0, "%s: type %d not recognized for l->type", \ "BINFUNC_F_OPERATOR_SET", l->type); \ } static gal_data_t * arithmetic_binary_function_flt(int operator, int flags, gal_data_t *l, gal_data_t *r) { int final_otype; gal_data_t *o=NULL; size_t out_size, minmapsize; /* Simple sanity check on the input sizes */ if( !( (flags & GAL_ARITHMETIC_NUMOK) && (l->size==1 || r->size==1)) && gal_data_dsize_is_different(l, r) ) error(EXIT_FAILURE, 0, "%s: the input datasets don't have the same " "dimension/size", __func__); /* Check for the types of the left and right operands. */ arithmetic_check_float_input(l, operator, "first"); arithmetic_check_float_input(r, operator, "second"); /* Set the output type. */ final_otype = gal_type_out(l->type, r->type); /* Set the output sizes. */ minmapsize = ( l->minmapsize < r->minmapsize ? l->minmapsize : r->minmapsize ); out_size = l->size > r->size ? l->size : r->size; /* If we want inplace output, set the output pointer to one input. Note that the output type can be different from both inputs. */ if(flags & GAL_ARITHMETIC_INPLACE) { if (l->type==final_otype && out_size==l->size) o = l; else if(r->type==final_otype && out_size==r->size) o = r; } /* If the output pointer was not set for any reason, allocate it. For `mmapsize', note that since its `size_t', it will always be Positive. The `-1' that is recommended to give when you want the value in RAM is actually the largest possible memory location. So we just have to choose the smaller minmapsize of the two to decide if the output array should be in RAM or not. */ if(o==NULL) o = gal_data_alloc(NULL, final_otype, l->size>1 ? l->ndim : r->ndim, l->size>1 ? l->dsize : r->dsize, l->size>1 ? l->wcs : r->wcs, 0, minmapsize, NULL, NULL, NULL); /* Start setting the operator and operands. */ switch(operator) { case GAL_ARITHMETIC_OP_POW: BINFUNC_F_OPERATOR_SET( pow ); break; default: error(EXIT_FAILURE, 0, "%s: operator code %d not recognized", __func__, operator); } /* Clean up. Note that if the input arrays can be freed, and any of right or left arrays needed conversion, `BINFUNC_CONVERT_TO_COMPILED_TYPE' has already freed the input arrays, and we only have `r' and `l' allocated in any case. Alternatively, when the inputs shouldn't be freed, the only allocated spaces are the `r' and `l' arrays if their types weren't compiled for binary operations, we can tell this from the pointers: if they are different from the original pointers, they were allocated. */ if(flags & GAL_ARITHMETIC_FREE) { if (o==l) gal_data_free(r); else if(o==r) gal_data_free(l); else { gal_data_free(l); gal_data_free(r); } } /* Return */ return o; } /**********************************************************************/ /**************** High-level functions *****************/ /**********************************************************************/ char * gal_arithmetic_operator_string(int operator) { switch(operator) { case GAL_ARITHMETIC_OP_PLUS: return "+"; case GAL_ARITHMETIC_OP_MINUS: return "-"; case GAL_ARITHMETIC_OP_MULTIPLY: return "*"; case GAL_ARITHMETIC_OP_DIVIDE: return "/"; case GAL_ARITHMETIC_OP_MODULO: return "%"; case GAL_ARITHMETIC_OP_LT: return "<"; case GAL_ARITHMETIC_OP_LE: return "<="; case GAL_ARITHMETIC_OP_GT: return ">"; case GAL_ARITHMETIC_OP_GE: return ">="; case GAL_ARITHMETIC_OP_EQ: return "=="; case GAL_ARITHMETIC_OP_NE: return "!="; case GAL_ARITHMETIC_OP_AND: return "and"; case GAL_ARITHMETIC_OP_OR: return "or"; case GAL_ARITHMETIC_OP_NOT: return "not"; case GAL_ARITHMETIC_OP_ISBLANK: return "isblank"; case GAL_ARITHMETIC_OP_WHERE: return "where"; case GAL_ARITHMETIC_OP_BITAND: return "bitand"; case GAL_ARITHMETIC_OP_BITOR: return "bitor"; case GAL_ARITHMETIC_OP_BITXOR: return "bitxor"; case GAL_ARITHMETIC_OP_BITLSH: return "lshift"; case GAL_ARITHMETIC_OP_BITRSH: return "rshift"; case GAL_ARITHMETIC_OP_BITNOT: return "bitnot"; case GAL_ARITHMETIC_OP_ABS: return "abs"; case GAL_ARITHMETIC_OP_POW: return "pow"; case GAL_ARITHMETIC_OP_SQRT: return "sqrt"; case GAL_ARITHMETIC_OP_LOG: return "log"; case GAL_ARITHMETIC_OP_LOG10: return "log10"; case GAL_ARITHMETIC_OP_MINVAL: return "minvalue"; case GAL_ARITHMETIC_OP_MAXVAL: return "maxvalue"; case GAL_ARITHMETIC_OP_NUMVAL: return "numvalue"; case GAL_ARITHMETIC_OP_SUMVAL: return "sumvalue"; case GAL_ARITHMETIC_OP_MEANVAL: return "meanvalue"; case GAL_ARITHMETIC_OP_STDVAL: return "stdvalue"; case GAL_ARITHMETIC_OP_MEDIANVAL: return "medianvalue"; case GAL_ARITHMETIC_OP_MIN: return "min"; case GAL_ARITHMETIC_OP_MAX: return "max"; case GAL_ARITHMETIC_OP_NUM: return "num"; case GAL_ARITHMETIC_OP_SUM: return "sum"; case GAL_ARITHMETIC_OP_MEAN: return "mean"; case GAL_ARITHMETIC_OP_STD: return "std"; case GAL_ARITHMETIC_OP_MEDIAN: return "median"; case GAL_ARITHMETIC_OP_TO_UINT8: return "uchar"; case GAL_ARITHMETIC_OP_TO_INT8: return "char"; case GAL_ARITHMETIC_OP_TO_UINT16: return "ushort"; case GAL_ARITHMETIC_OP_TO_INT16: return "short"; case GAL_ARITHMETIC_OP_TO_UINT32: return "uint"; case GAL_ARITHMETIC_OP_TO_INT32: return "int"; case GAL_ARITHMETIC_OP_TO_UINT64: return "ulong"; case GAL_ARITHMETIC_OP_TO_INT64: return "long"; case GAL_ARITHMETIC_OP_TO_FLOAT32: return "float32"; case GAL_ARITHMETIC_OP_TO_FLOAT64: return "float64"; default: error(EXIT_FAILURE, 0, "%s: operator code %d not recognized", __func__, operator); } error(EXIT_FAILURE, 0, "%s: a bug! Please contact us to fix the problem. " "Control has reached the end of this function. This should not have " "happened", __func__); return NULL; } gal_data_t * gal_arithmetic(int operator, int flags, ...) { va_list va; gal_data_t *d1, *d2, *d3, *out=NULL; /* Prepare the variable arguments (starting after the flags argument). */ va_start(va, flags); /* Depending on the operator do the job: */ switch(operator) { /* Binary operators with any data type. */ case GAL_ARITHMETIC_OP_PLUS: case GAL_ARITHMETIC_OP_MINUS: case GAL_ARITHMETIC_OP_MULTIPLY: case GAL_ARITHMETIC_OP_DIVIDE: case GAL_ARITHMETIC_OP_LT: case GAL_ARITHMETIC_OP_LE: case GAL_ARITHMETIC_OP_GT: case GAL_ARITHMETIC_OP_GE: case GAL_ARITHMETIC_OP_EQ: case GAL_ARITHMETIC_OP_NE: case GAL_ARITHMETIC_OP_AND: case GAL_ARITHMETIC_OP_OR: d1 = va_arg(va, gal_data_t *); d2 = va_arg(va, gal_data_t *); out=arithmetic_binary(operator, flags, d1, d2); break; case GAL_ARITHMETIC_OP_NOT: d1 = va_arg(va, gal_data_t *); out=arithmetic_not(d1, flags); break; case GAL_ARITHMETIC_OP_ISBLANK: d1 = va_arg(va, gal_data_t *); out = gal_blank_flag(d1); if(flags & GAL_ARITHMETIC_FREE) gal_data_free(d1); break; case GAL_ARITHMETIC_OP_WHERE: d1 = va_arg(va, gal_data_t *); /* To modify value/array. */ d2 = va_arg(va, gal_data_t *); /* Condition (unsigned char). */ d3 = va_arg(va, gal_data_t *); /* If true value/array. */ arithmetic_where(flags, d1, d2, d3); out=d1; break; /* Unary function operators. */ case GAL_ARITHMETIC_OP_SQRT: case GAL_ARITHMETIC_OP_LOG: case GAL_ARITHMETIC_OP_LOG10: d1 = va_arg(va, gal_data_t *); out=arithmetic_unary_function(operator, flags, d1); break; /* Statistical operators that return one value. */ case GAL_ARITHMETIC_OP_MINVAL: case GAL_ARITHMETIC_OP_MAXVAL: case GAL_ARITHMETIC_OP_NUMVAL: case GAL_ARITHMETIC_OP_SUMVAL: case GAL_ARITHMETIC_OP_MEANVAL: case GAL_ARITHMETIC_OP_STDVAL: case GAL_ARITHMETIC_OP_MEDIANVAL: d1 = va_arg(va, gal_data_t *); out=arithmetic_from_statistics(operator, flags, d1); break; /* Absolute operator */ case GAL_ARITHMETIC_OP_ABS: d1 = va_arg(va, gal_data_t *); out=arithmetic_abs(flags, d1); break; /* Multi-operand operators */ case GAL_ARITHMETIC_OP_MIN: case GAL_ARITHMETIC_OP_MAX: case GAL_ARITHMETIC_OP_NUM: case GAL_ARITHMETIC_OP_SUM: case GAL_ARITHMETIC_OP_MEAN: case GAL_ARITHMETIC_OP_STD: case GAL_ARITHMETIC_OP_MEDIAN: d1 = va_arg(va, gal_data_t *); out=arithmetic_multioperand(operator, flags, d1); break; /* Binary function operators. */ case GAL_ARITHMETIC_OP_POW: d1 = va_arg(va, gal_data_t *); d2 = va_arg(va, gal_data_t *); out=arithmetic_binary_function_flt(operator, flags, d1, d2); break; /* Binary operators that only work on integer types. */ case GAL_ARITHMETIC_OP_BITAND: case GAL_ARITHMETIC_OP_BITOR: case GAL_ARITHMETIC_OP_BITXOR: case GAL_ARITHMETIC_OP_BITLSH: case GAL_ARITHMETIC_OP_BITRSH: case GAL_ARITHMETIC_OP_MODULO: d1 = va_arg(va, gal_data_t *); d2 = va_arg(va, gal_data_t *); out=arithmetic_binary(operator, flags, d1, d2); break; case GAL_ARITHMETIC_OP_BITNOT: d1 = va_arg(va, gal_data_t *); out=arithmetic_bitwise_not(flags, d1); break; /* Conversion operators. */ case GAL_ARITHMETIC_OP_TO_UINT8: case GAL_ARITHMETIC_OP_TO_INT8: case GAL_ARITHMETIC_OP_TO_UINT16: case GAL_ARITHMETIC_OP_TO_INT16: case GAL_ARITHMETIC_OP_TO_UINT32: case GAL_ARITHMETIC_OP_TO_INT32: case GAL_ARITHMETIC_OP_TO_UINT64: case GAL_ARITHMETIC_OP_TO_INT64: case GAL_ARITHMETIC_OP_TO_FLOAT32: case GAL_ARITHMETIC_OP_TO_FLOAT64: d1 = va_arg(va, gal_data_t *); out=arithmetic_change_type(d1, operator, flags); break; /* When the operator is not recognized. */ default: error(EXIT_FAILURE, 0, "%s: the argument \"%d\" could not be " "interpretted as an operator", __func__, operator); } /* End the variable argument structure and return. */ va_end(va); return out; } gnuastro-0.5/lib/Makefile.in0000644000175000017500000023503613217217706012773 00000000000000# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software 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= @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ 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See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Necessary flags. ## ## $(top_srcdir)/bootstrapped/lib: only necessary for the libraries since ## the Gnulib functions will be statically linked to the Gnuastro ## library so linking to Gnuastro is enough to access them also. ## ## SYSCONFIG_DIR: only necessary in `options.c' to get the system ## installation directory. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib \ -DSYSCONFIG_DIR=\"$(sysconfdir)\" # Define the main compiled library file, its Libtool version and also link # with Gnulib's compiled library for this system. We are doing this so the # Gnuastro library functions can also benefit from Gnulib's many great # features. 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Headers are only mentioned within the source files, # and if they are not explicitly mentioned somewhere in the Makefile, they # will not distributed, so we need to explicitly tell Automake to # distribute them here. internaldir=$(top_srcdir)/lib/gnuastro-internal EXTRA_DIST = gnuastro.pc.in $(headersdir)/README $(internaldir)/README \ $(internaldir)/arithmetic-and.h $(internaldir)/arithmetic-binary.h \ $(internaldir)/arithmetic-bitand.h $(internaldir)/arithmetic-bitlsh.h \ $(internaldir)/arithmetic-bitor.h $(internaldir)/arithmetic-bitrsh.h \ $(internaldir)/arithmetic-bitxor.h $(internaldir)/arithmetic-divide.h \ $(internaldir)/arithmetic-eq.h $(internaldir)/arithmetic-ge.h \ $(internaldir)/arithmetic-gt.h $(internaldir)/arithmetic-internal.h \ $(internaldir)/arithmetic-le.h $(internaldir)/arithmetic-lt.h \ $(internaldir)/arithmetic-minus.h $(internaldir)/arithmetic-modulo.h \ $(internaldir)/arithmetic-multiply.h $(internaldir)/arithmetic-ne.h \ $(internaldir)/arithmetic-or.h $(internaldir)/arithmetic-plus.h \ $(internaldir)/checkset.h $(internaldir)/commonopts.h \ $(internaldir)/config.h.in $(internaldir)/fixedstringmacros.h \ $(internaldir)/options.h $(internaldir)/tableintern.h \ $(internaldir)/timing.h # Definitions for Gnuastro's the pkg-config file (inspired from GSL's # Makefile.am) pkgconfig_DATA = gnuastro.pc pkgconfigdir = $(libdir)/pkgconfig CLEANFILES = gnuastro.pc gnuastro/config.h # Build `gnuastro/config.h' based on the information in the Makefile after # the Makefile has been built. gnuastro/config.h: Makefile $(internaldir)/config.h.in rm -f $@ $@.tmp $(MKDIR_P) gnuastro $(SED) -e 's|@VERSION[@]|$(VERSION)|g' \ -e 's|@HAVE_LIBGIT2[@]|$(HAVE_LIBGIT2)|g' \ -e 's|@HAVE_WCSLIB_VERSION[@]|$(HAVE_WCSLIB_VERSION)|g' \ -e 's|@HAVE_PTHREAD_BARRIER[@]|$(HAVE_PTHREAD_BARRIER)|g' \ -e 's|@SIZEOF_LONG[@]|$(SIZEOF_LONG)|g' \ -e 's|@SIZEOF_SIZE_T[@]|$(SIZEOF_SIZE_T)|g' \ -e 's|@RESTRICT_REPLACEMENT[@]|$(RESTRICT_REPLACEMENT)|g' \ $(internaldir)/config.h.in >> $@.tmp chmod a-w $@.tmp mv $@.tmp $@ # Build Gnuastro's pkg-config file similar to `gnuastro/config.h'. gnuastro.pc: Makefile $(srcdir)/gnuastro.pc.in rm -f $@ $@.tmp $(SED) \ -e 's|@prefix[@]|$(prefix)|g' \ -e 's|@exec_prefix[@]|$(exec_prefix)|g' \ -e 's|@libdir[@]|$(libdir)|g' \ -e 's|@includedir[@]|$(includedir)|g' \ -e 's|@LIBS[@]|$(LIBS)|g' \ -e 's|@VERSION[@]|$(VERSION)|g' \ '$(srcdir)/$@.in' >> $@.tmp chmod a-w $@.tmp mv $@.tmp $@ # Remove the two local directories we needed during installation from the # library search paths of the installed `libgnuastro.la'. # # Note that this hook is executed after every installation command # (including `make uninstall'). So we should only do it if the library # actually exists. install-exec-hook: if [ -f $(libdir)/libgnuastro.la ]; then \ $(SED) -e 's/ -L..\/lib//g' -e 's/ -L..\/..\/lib//g' \ $(libdir)/libgnuastro.la > libgnuastro.la_tmp; \ mv libgnuastro.la_tmp $(libdir)/libgnuastro.la; \ fi gnuastro-0.5/lib/gnuastro-internal/0000755000175000017500000000000013217220466014446 500000000000000gnuastro-0.5/lib/gnuastro-internal/timing.h0000644000175000017500000000357113121462410016023 00000000000000/********************************************************************* Functions to report timing in verbose mode. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TIMING_H__ #define __GAL_TIMING_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ #define GAL_TIMING_VERB_MSG_LENGTH_V 50 #define GAL_TIMING_VERB_MSG_LENGTHS_2_V 65 long gal_timing_time_based_rng_seed(); void gal_timing_report(struct timeval *t1, char *jobname, size_t level); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TIMING_H__ */ gnuastro-0.5/lib/gnuastro-internal/tableintern.h0000644000175000017500000000605113121462410017037 00000000000000/********************************************************************* tableintern -- Internalfunctions for table input and output. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TABLEINTERN_H__ #define __GAL_TABLEINTERN_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* Includes `gnuastro/data.h' and `fitsio.h' */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /************************************************************************/ /*************** Error messages ***************/ /************************************************************************/ void gal_tableintern_error_col_selection(char *filename, char *hdu, char *errorstring); /************************************************************************/ /*************** Formats ***************/ /************************************************************************/ uint8_t gal_tableintern_string_to_format(char *string); char * gal_tableintern_format_as_string(uint8_t tableformat); uint8_t gal_tableintern_string_to_searchin(char *string); char * gal_tableintern_searchin_as_string(uint8_t searchin); void gal_tableintern_check_fits_format(char *filename, int tableformat); /************************************************************************/ /*************** Printing information ***************/ /************************************************************************/ void gal_tableintern_col_print_info(gal_data_t *col, int tableformat, char *fmt, char *lng); void gal_tableintern_read_blank(gal_data_t *col, char *blank); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TABLE_H__ */ gnuastro-0.5/lib/gnuastro-internal/options.h0000644000175000017500000002607313216276304016243 00000000000000/********************************************************************* Function to parse options and configuration file values. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_OPTIONS_H__ #define __GAL_OPTIONS_H__ #include #include #include /**********************************************************************/ /************ Common options ***************/ /**********************************************************************/ /* Type for options that don't accept an argument/value. This macro is defined to help make the definition and processing of these options easier and less buggy. Please use this macro for such options. */ #define GAL_OPTIONS_NO_ARG_TYPE GAL_TYPE_UINT8 /* When printing the option names, values and comments, we want things to be clean and readable (all the comments starting on one line for most, ideally all, lines). But in some cases, option values can become too long (for example the `--polygon' option in Crop, which takes many coordinates). So simply using the maximum option length is going to make the whole thing unreadable and we need to have a maximum so this rule only applies to them. */ #define GAL_OPTIONS_MAX_VALUE_LEN 10 /* Statically allocated space for printing option values. */ #define GAL_OPTIONS_STATIC_MEM_FOR_VALUES 2000 /* Standard groups of options. From the Argp manual (in GNU C Library): "In a long help message, options are sorted alphabetically within each group, and the groups presented in the order 0, 1, 2, ..., N, -M, ..., -2, -1." We want the Operating mode group of options to be the last and the input and output groups to the be the first. So first we set the operating mdoe group code to `-1', and benefit from the definition of the Enumerator type in C, so each field afterwards will be one integer larger than the previous. The largest common option group is then used to build the codes of program-specific option groups. */ enum options_standard_groups { GAL_OPTIONS_GROUP_OPERATING_MODE = -1, GAL_OPTIONS_GROUP_INPUT=1, GAL_OPTIONS_GROUP_TESSELLATION, GAL_OPTIONS_GROUP_OUTPUT, GAL_OPTIONS_GROUP_AFTER_COMMON, }; /* Key values for the common options, the free alphabetical keys are listed below. You can use any of the free letters for an option in a program. Note that `-V', which is used by GNU and implemented by Argp, is also removed from this list. a b c d e f g i j k l m n p r s t u v w x y z A B C E G H J L O Q R W X Y */ enum options_common_keys { /* With short-option version */ GAL_OPTIONS_KEY_HDU = 'h', GAL_OPTIONS_KEY_OUTPUT = 'o', GAL_OPTIONS_KEY_TYPE = 'T', GAL_OPTIONS_KEY_DONTDELETE = 'D', GAL_OPTIONS_KEY_KEEPINPUTDIR = 'K', GAL_OPTIONS_KEY_QUIET = 'q', GAL_OPTIONS_KEY_NUMTHREADS = 'N', GAL_OPTIONS_KEY_PRINTPARAMS = 'P', GAL_OPTIONS_KEY_SETDIRCONF = 'S', GAL_OPTIONS_KEY_SETUSRCONF = 'U', GAL_OPTIONS_KEY_IGNORECASE = 'I', GAL_OPTIONS_KEY_TILESIZE = 'Z', GAL_OPTIONS_KEY_NUMCHANNELS = 'M', GAL_OPTIONS_KEY_REMAINDERFRAC = 'F', /* Only long option (integers for keywords). */ GAL_OPTIONS_KEY_MINMAPSIZE = 500, GAL_OPTIONS_KEY_LOG, GAL_OPTIONS_KEY_CITE, GAL_OPTIONS_KEY_CONFIG, GAL_OPTIONS_KEY_SEARCHIN, GAL_OPTIONS_KEY_LASTCONFIG, GAL_OPTIONS_KEY_TABLEFORMAT, GAL_OPTIONS_KEY_ONLYVERSION, GAL_OPTIONS_KEY_WORKOVERCH, GAL_OPTIONS_KEY_CHECKTILES, GAL_OPTIONS_KEY_ONEELEMPERTILE, GAL_OPTIONS_KEY_INTERPONLYBLANK, GAL_OPTIONS_KEY_INTERPNUMNGB, }; /* Conditions to check */ enum gal_options_range_values { GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_RANGE_GE_0_LT_1, GAL_OPTIONS_RANGE_GT_0_LT_1, GAL_OPTIONS_RANGE_GT_0_ODD, GAL_OPTIONS_RANGE_0_OR_ODD, }; /* What to do if option isn't given. Note that in each program's `main.c' the main program structure is initialized to zero (or NULL for pointers). */ enum gal_options_mandatory_values { GAL_OPTIONS_NOT_MANDATORY, /* =0 in C standard. */ GAL_OPTIONS_MANDATORY, }; /* If the option has already been given a value or not. */ enum gal_options_set_values { GAL_OPTIONS_NOT_SET, /* =0 in C standard. */ GAL_OPTIONS_SET, }; /* The structure keeping all the values of the common options in Gnuastro's programs. */ struct gal_options_common_params { /* Tessellation. */ struct gal_tile_two_layer_params tl; /* Two layer tessellation params. */ uint8_t interponlyblank; /* Only interpolate over blank values. */ size_t interpnumngb; /* Number of neighbors for interpolation. */ /* Input. */ char *hdu; /* Image extension. */ uint8_t searchin; /* Column meta-data to match/search. */ uint8_t ignorecase; /* Ignore case when matching col info. */ /* Output. */ char *output; /* Directory containg output. */ uint8_t type; /* Data type of output. */ uint8_t dontdelete; /* ==1: Don't delete existing file. */ uint8_t keepinputdir; /* Keep input directory for auto output. */ uint8_t tableformat; /* Internal code for output table format. */ /* Operating modes. */ uint8_t quiet; /* Only print errors. */ size_t numthreads; /* Number of threads to use. */ size_t minmapsize; /* Minimum bytes necessary to use mmap. */ uint8_t log; /* Make a log file. */ /* Configuration files. */ uint8_t printparams; /* To print the full list of parameters. */ uint8_t setdirconf; /* To write the directory config file. */ uint8_t setusrconf; /* To write teh user config config file. */ uint8_t lastconfig; /* This is the last configuration file. */ /* For internal (to option processing) purposes. */ uint8_t keep; /* Output file can exist. */ void *program_struct; /* Host program's main variable struct. */ char *program_name; /* Official name to be used in text. */ char *program_exec; /* Program's executable name. */ char *program_bibtex; /* BibTeX record for this program. */ char *program_authors; /* List of the program authors. */ struct argp_option *coptions; /* Common options to all programs. */ struct argp_option *poptions; /* Program specific options. */ gal_list_i32_t *mand_common; /* Common mandatory options. */ gal_list_str_t *novalue_doc; /* Mandatory opts, no value */ gal_list_str_t *novalue_name; /* Mandatory opts, no value */ }; /**********************************************************************/ /************ Option utilities ***************/ /**********************************************************************/ int gal_options_is_last(struct argp_option *option); int gal_options_is_category_title(struct argp_option *option); void gal_options_add_to_not_given(struct gal_options_common_params *cp, struct argp_option *option); void gal_options_abort_if_mandatory_missing(struct gal_options_common_params *cp); /**********************************************************************/ /************ Parser functions for common options ***************/ /**********************************************************************/ void * gal_options_check_version(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); void * gal_options_print_citation(struct argp_option *option, char *arg, char *filename, size_t lineno, void *pa); void * gal_options_read_type(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); void * gal_options_read_searchin(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); void * gal_options_read_tableformat(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); gal_data_t * gal_options_parse_list_of_numbers(char *string, char *filename, size_t lineno); gal_data_t * gal_options_parse_csv_strings_raw(char *string, char *filename, size_t lineno); void * gal_options_parse_csv_strings(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); void * gal_options_parse_sizes_reverse(struct argp_option *option, char *arg, char *filename, size_t lineno, void *params); void * gal_options_parse_csv_float64(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); void * gal_options_read_sigma_clip(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk); /**********************************************************************/ /************ Command-line options ***************/ /**********************************************************************/ error_t gal_options_set_from_key(int key, char *arg, struct argp_option *options, struct gal_options_common_params *cp); error_t gal_options_common_argp_parse(int key, char *arg, struct argp_state *state); /**********************************************************************/ /************ Configuration files ***************/ /**********************************************************************/ void * gal_options_call_parse_config_file(struct argp_option *option, char *arg, char *filename, size_t lineno, void *cp); void gal_options_read_config_set(struct gal_options_common_params *cp); /**********************************************************************/ /************ Printing/Writing ***************/ /**********************************************************************/ void gal_options_print_state(struct gal_options_common_params *cp); #endif gnuastro-0.5/lib/gnuastro-internal/fixedstringmacros.h0000644000175000017500000000611213121462410020261 00000000000000/********************************************************************* Fixed strings for use in all utilities. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_FIXEDSTRINGMACROS_H__ #define __GAL_FIXEDSTRINGMACROS_H__ #define GAL_STRINGS_SHORT_COPYRIGHT \ "Copyright (C) 2015-2017, Free Software Foundation, Inc." #define GAL_STRINGS_SHORT_LICENSE \ "License GPLv3+: GNU General public license version 3 or later." #define GAL_STRINGS_COPYRIGHT \ GAL_STRINGS_SHORT_COPYRIGHT"\n"GAL_STRINGS_SHORT_LICENSE"\n" \ "This is free software: you are free to change and redistribute " \ "it.\nThere is NO WARRANTY, to the extent permitted by law." \ #define GAL_STRINGS_TOP_HELP_INFO \ "\n"PROGRAM_NAME" is part of "PACKAGE_STRING".\n" /* This is fixed for all the packages. */ #define GAL_STRINGS_MORE_HELP_INFO \ "\nFor more information, please run any of the " \ "following commands. In particular the second contains a very " \ "comprehensive explanation of "PROGRAM_NAME"'s invocation: expected " \ "input(s), output(s), and a full description of all the options.\n\n" \ " All options and their values: $ "PROGRAM_EXEC" -P\n" \ " Inputs/Outputs and options: $ info "PROGRAM_EXEC"\n" \ " Full section in manual/book: $ info "PROGRAM_NAME"\n" \ " Full Gnuastro manual/book: $ info "PACKAGE_TARNAME"\n\n" \ "If you couldn't find your answer in the manual, you can get " \ "direct help from experienced Gnuastro users and developers. " \ "For more information, please run:\n\n" \ " $ info help-gnuastro\n\n" \ PROGRAM_NAME" options:" \ /* This can be used in the end of error messages related to option values. */ #define GAL_STRINGS_HOW_TO_CHECK_VALUES \ " You can check all the input values with the `--printparams' " \ "(-P) option." #endif /* __GAL_FIXEDSTRINGMACROS_H__ */ gnuastro-0.5/lib/gnuastro-internal/config.h.in0000644000175000017500000000540013125235120016377 00000000000000/********************************************************************* Functions dealing with general aspects of all Gnuastro. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_CONFIG_H__ #define __GAL_CONFIG_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* The restrict keyword might not be present on some systems, so we are redefining it here based on the checks in `configure.ac', see there for more comments. */ #define restrict @RESTRICT_REPLACEMENT@ /* Configuration macros: */ #define GAL_CONFIG_VERSION "@VERSION@" #define GAL_CONFIG_HAVE_LIBGIT2 @HAVE_LIBGIT2@ #define GAL_CONFIG_HAVE_WCSLIB_VERSION @HAVE_WCSLIB_VERSION@ #define GAL_CONFIG_HAVE_PTHREAD_BARRIER @HAVE_PTHREAD_BARRIER@ #define GAL_CONFIG_BIN_OP_UINT8 @HAVE_BIN_OP_UINT8@ #define GAL_CONFIG_BIN_OP_INT8 @HAVE_BIN_OP_INT8@ #define GAL_CONFIG_BIN_OP_UINT16 @HAVE_BIN_OP_UINT16@ #define GAL_CONFIG_BIN_OP_INT16 @HAVE_BIN_OP_INT16@ #define GAL_CONFIG_BIN_OP_UINT32 @HAVE_BIN_OP_UINT32@ #define GAL_CONFIG_BIN_OP_INT32 @HAVE_BIN_OP_INT32@ #define GAL_CONFIG_BIN_OP_UINT64 @HAVE_BIN_OP_UINT64@ #define GAL_CONFIG_BIN_OP_INT64 @HAVE_BIN_OP_INT64@ #define GAL_CONFIG_BIN_OP_FLOAT32 @HAVE_BIN_OP_FLOAT32@ #define GAL_CONFIG_BIN_OP_FLOAT64 @HAVE_BIN_OP_FLOAT64@ #define GAL_CONFIG_SIZEOF_LONG @SIZEOF_LONG@ #define GAL_CONFIG_SIZEOF_SIZE_T @SIZEOF_SIZE_T@ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_CONFIG_H__ */ gnuastro-0.5/lib/gnuastro-internal/commonopts.h0000644000175000017500000002463713164537456016764 00000000000000/********************************************************************* Common parameters between all programs. IMPORTANT: This header must only be included the programs, not libraries. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_COMMONOPTS_H__ #define __GAL_COMMONOPTS_H__ /* Common options for all programs. IMPORTANT NOTE: This header should only be included in the programs, not the libraries, and in particular `options.c'. Because we want each program to have its own allocation of the common options structure. If it is included in options.c, then it will be shared between all the programs. */ struct argp_option gal_commonopts_options[] = { { 0, 0, 0, 0, "Input:", GAL_OPTIONS_GROUP_INPUT }, { "hdu", GAL_OPTIONS_KEY_HDU, "STR/INT", 0, "Extension name or number of input data.", GAL_OPTIONS_GROUP_INPUT, &cp->hdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "searchin", GAL_OPTIONS_KEY_SEARCHIN, "STR", 0, "Select column(s) in: `name', `unit', `comment'.", GAL_OPTIONS_GROUP_INPUT, &cp->searchin, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_read_searchin }, { "ignorecase", GAL_OPTIONS_KEY_IGNORECASE, 0, 0, "Ignore case in matching/searching columns.", GAL_OPTIONS_GROUP_INPUT, &cp->ignorecase, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Tile grid (tessellation) options. */ { 0, 0, 0, 0, "Tessellation (tile grid):", GAL_OPTIONS_GROUP_TESSELLATION }, { "tilesize", GAL_OPTIONS_KEY_TILESIZE, "INT[,INT]", 0, "Regular tile size on dim.s (FITS order).", GAL_OPTIONS_GROUP_TESSELLATION, &cp->tl.tilesize, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_sizes_reverse }, { "numchannels", GAL_OPTIONS_KEY_NUMCHANNELS, "INT[,..]", 0, "No. of channels in dim.s (FITS order).", GAL_OPTIONS_GROUP_TESSELLATION, &cp->tl.numchannels, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_sizes_reverse }, { "remainderfrac", GAL_OPTIONS_KEY_REMAINDERFRAC, "FLT", 0, "Fraction of remainder to split last tile.", GAL_OPTIONS_GROUP_TESSELLATION, &cp->tl.remainderfrac, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0_LT_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, }, { "workoverch", GAL_OPTIONS_KEY_WORKOVERCH, 0, 0, "Work (not tile) over channel edges.", GAL_OPTIONS_GROUP_TESSELLATION, &cp->tl.workoverch, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checktiles", GAL_OPTIONS_KEY_CHECKTILES, 0, 0, "Tile IDs in an image, the size of input.", GAL_OPTIONS_GROUP_TESSELLATION, &cp->tl.checktiles, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "oneelempertile", GAL_OPTIONS_KEY_ONEELEMPERTILE, 0, 0, "Display 1 element/tile, not full input res.", GAL_OPTIONS_GROUP_TESSELLATION, &cp->tl.oneelempertile, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "interponlyblank", GAL_OPTIONS_KEY_INTERPONLYBLANK, 0, 0, "Only interpolate over the blank tiles.", GAL_OPTIONS_GROUP_TESSELLATION, &cp->interponlyblank, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "interpnumngb", GAL_OPTIONS_KEY_INTERPNUMNGB, "INT", 0, "No. of neighbors to use for interpolation.", GAL_OPTIONS_GROUP_TESSELLATION, &cp->interpnumngb, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Output:", GAL_OPTIONS_GROUP_OUTPUT }, { "output", GAL_OPTIONS_KEY_OUTPUT, "STR", 0, "Output name.", GAL_OPTIONS_GROUP_OUTPUT, &cp->output, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "type", GAL_OPTIONS_KEY_TYPE, "STR", 0, "Type of output: e.g., int16, float32, etc...", GAL_OPTIONS_GROUP_OUTPUT, &cp->type, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_read_type }, { "tableformat", GAL_OPTIONS_KEY_TABLEFORMAT, "STR", 0, "Table format: `fits-ascii', `fits-binary'.", GAL_OPTIONS_GROUP_OUTPUT, &cp->tableformat, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_read_tableformat }, { "dontdelete", GAL_OPTIONS_KEY_DONTDELETE, 0, 0, "Don't delete output if it exists.", GAL_OPTIONS_GROUP_OUTPUT, &cp->dontdelete, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "keepinputdir", GAL_OPTIONS_KEY_KEEPINPUTDIR, 0, 0, "Keep input directory for automatic output.", GAL_OPTIONS_GROUP_OUTPUT, &cp->keepinputdir, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Operating modes:", GAL_OPTIONS_GROUP_OPERATING_MODE }, { "quiet", GAL_OPTIONS_KEY_QUIET, 0, 0, "Only report errors, remain quiet about steps.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->quiet, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "numthreads", GAL_OPTIONS_KEY_NUMTHREADS, "INT", 0, "Number of CPU threads to use.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->numthreads, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "minmapsize", GAL_OPTIONS_KEY_MINMAPSIZE, "INT", 0, "Minimum bytes in array to not use ram RAM.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->minmapsize, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "log", GAL_OPTIONS_KEY_LOG, 0, 0, "Information about output(s) in a log file.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->log, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Internal (before control goes back to the program). */ { "cite", GAL_OPTIONS_KEY_CITE, 0, 0, "BibTeX citation for this program.", GAL_OPTIONS_GROUP_OPERATING_MODE, NULL, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_print_citation }, { "printparams", GAL_OPTIONS_KEY_PRINTPARAMS, 0, 0, "Print parameter values to be used and abort.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->printparams, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "config", GAL_OPTIONS_KEY_CONFIG, "STR", 0, "Read configuration file STR immediately.", GAL_OPTIONS_GROUP_OPERATING_MODE, NULL, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_call_parse_config_file }, { "setdirconf", GAL_OPTIONS_KEY_SETDIRCONF, 0, 0, "Set default values for this directory and abort.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->setdirconf, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "setusrconf", GAL_OPTIONS_KEY_SETUSRCONF, 0, 0, "Set default values for this user and abort.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->setusrconf, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "lastconfig", GAL_OPTIONS_KEY_LASTCONFIG, 0, 0, "Do not parse any more configuration files.", GAL_OPTIONS_GROUP_OPERATING_MODE, &cp->lastconfig, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "onlyversion", GAL_OPTIONS_KEY_ONLYVERSION, "STR", 0, "Only run if the program version is STR.", GAL_OPTIONS_GROUP_OPERATING_MODE, NULL, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_check_version }, {0} }; #endif gnuastro-0.5/lib/gnuastro-internal/checkset.h0000644000175000017500000000654713211076737016350 00000000000000/********************************************************************* Functions to check and set command line argument values and files. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_CHECKSET_H__ #define __GAL_CHECKSET_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /**************************************************************/ /********** Check fixed strings ************/ /**************************************************************/ void gal_checkset_known_types(char *optarg, int *type, char *filename, size_t lineno); /**************************************************************/ /********** My String functions: ************/ /**************************************************************/ int gal_checkset_string_has_space(char *in); char * gal_checkset_malloc_cat(char *inname, char *toappend); void gal_checkset_allocate_copy(const char *arg, char **copy); void gal_checkset_allocate_copy_set(char *arg, char **copy, int *set); char * gal_checkset_dataset_name(char *filename, char *hdu); /**************************************************************/ /********** Set file names and check if they exist ************/ /**************************************************************/ char * gal_checkset_dir_part(char *filename); char * gal_checkset_not_dir_part(char *filename); void gal_checkset_check_file(char *filename); int gal_checkset_check_file_return(char *filename); void /* keep==0 && dontdelete==0: file will be deleted if exists.*/ gal_checkset_writable_remove(char *filename, int keep, int dontdelete); int gal_checkset_dir_0_file_1(char *name, int dontdelete); char * gal_checkset_automatic_output(struct gal_options_common_params *cp, char *inname, char *suffix); void gal_checkset_check_dir_write_add_slash(char **dirname); void gal_checkset_mkdir(char *dirname); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_CHECKSET_H__ */ gnuastro-0.5/lib/gnuastro-internal/arithmetic-plus.h0000644000175000017500000000213413215601241017641 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_PLUS_H__ #define __ARITHMETIC_PLUS_H__ void arithmetic_plus(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-or.h0000644000175000017500000000212613215601241017277 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_OR_H__ #define __ARITHMETIC_OR_H__ void arithmetic_or(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-ne.h0000644000175000017500000000212613215601241017261 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_NE_H__ #define __ARITHMETIC_NE_H__ void arithmetic_ne(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-multiply.h0000644000175000017500000000215013215601241020533 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_MULTIPLY_H__ #define __ARITHMETIC_MULTIPLY_H__ void arithmetic_multiply(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-modulo.h0000644000175000017500000000214213215601241020154 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_MODULO_H__ #define __ARITHMETIC_MODULO_H__ void arithmetic_modulo(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-minus.h0000644000175000017500000000213713215601241020014 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_MINUS_H__ #define __ARITHMETIC_MINUS_H__ void arithmetic_minus(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-lt.h0000644000175000017500000000212613215601241017276 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_LT_H__ #define __ARITHMETIC_LT_H__ void arithmetic_lt(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-le.h0000644000175000017500000000212613215601241017257 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_LE_H__ #define __ARITHMETIC_LE_H__ void arithmetic_le(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-internal.h0000644000175000017500000000477213215601241020504 00000000000000/********************************************************************* Arithmetic -- Preform arithmetic operations on datasets. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_ARITHMETIC_INTERNAL_H__ #define __GAL_ARITHMETIC_INTERNAL_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_CONFIG_ARITH_CHAR' and the rest of the types that we needed in the arithmetic function) is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro).*/ #ifndef IN_GNUASTRO_BUILD #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ int gal_arithmetic_binary_checkblank(gal_data_t *l, gal_data_t *r); char * gal_arithmetic_operator_string(int operator); gal_data_t * gal_arithmetic_convert_to_compiled_type(gal_data_t *in, int flags); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_ARITHMETIC_H__ */ gnuastro-0.5/lib/gnuastro-internal/arithmetic-gt.h0000644000175000017500000000212613215601241017271 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_GT_H__ #define __ARITHMETIC_GT_H__ void arithmetic_gt(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-ge.h0000644000175000017500000000212613215601241017252 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_GE_H__ #define __ARITHMETIC_GE_H__ void arithmetic_ge(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-eq.h0000644000175000017500000000212613215601241017264 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_EQ_H__ #define __ARITHMETIC_EQ_H__ void arithmetic_eq(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-divide.h0000644000175000017500000000214213215601241020121 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_DIVIDE_H__ #define __ARITHMETIC_DIVIDE_H__ void arithmetic_divide(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-bitxor.h0000644000175000017500000000214213215601241020164 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_BITXOR_H__ #define __ARITHMETIC_BITXOR_H__ void arithmetic_bitxor(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-bitrsh.h0000644000175000017500000000214213215601241020150 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_BITRSH_H__ #define __ARITHMETIC_BITRSH_H__ void arithmetic_bitrsh(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-bitor.h0000644000175000017500000000213713215601241020000 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_BITOR_H__ #define __ARITHMETIC_BITOR_H__ void arithmetic_bitor(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-bitlsh.h0000644000175000017500000000214213215601241020142 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_BITLSH_H__ #define __ARITHMETIC_BITLSH_H__ void arithmetic_bitlsh(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-bitand.h0000644000175000017500000000214213215601241020116 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_BITAND_H__ #define __ARITHMETIC_BITAND_H__ void arithmetic_bitand(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-binary.h0000644000175000017500000003135513215601241020151 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_BINARY_H__ #define __ARITHMETIC_BINARY_H__ /************************************************************************/ /************* Low-level operators *****************/ /************************************************************************/ /* Final step to be used by all operators and all types. */ #define BINARY_OP_OT_RT_LT_SET(OP, OT, LT, RT) { \ LT lb, *la=l->array; \ RT rb, *ra=r->array; \ OT ob, *oa=o->array, *of=oa + o->size; \ if(checkblank) \ { \ gal_blank_write(&lb, l->type); \ gal_blank_write(&rb, r->type); \ gal_blank_write(&ob, o->type); \ do \ { \ if(lb==lb && rb==rb)/* Both are integers. */ \ *oa = (*la!=lb && *ra!=rb) ? *la OP *ra : ob ; \ else if(lb==lb) /* Only left operand is an integer. */ \ *oa = (*la!=lb && *ra==*ra) ? *la OP *ra : ob; \ else /* Only right operand is an integer. */ \ *oa = (*la==*la && *ra!=rb) ? *la OP *ra : ob; \ if(l->size>1) ++la; \ if(r->size>1) ++ra; \ } \ while(++oasize==r->size) do *oa = *la++ OP *ra++; while(++oasize==1) do *oa = *la OP *ra++; while(++oaarray; \ RT *ra=r->array; \ OT *oa=o->array, *of=oa + o->size; \ if(l->size==r->size) do *oa = *la++ OP *ra++; while(++oasize==1) do *oa = *la OP *ra++; while(++oaarray; \ RT *ra=r->array; \ OT *oa=o->array, *of=oa + o->size; \ if(l->size==r->size) do {*oa = *la++ OP *ra; ++ra;} while(++oasize==1) do {*oa = *la OP *ra; ++ra;} while(++oatype) \ { \ case GAL_TYPE_UINT8: BINARY_SET_OUT_INT( F, OP, LT, uint8_t ) break; \ case GAL_TYPE_INT8: BINARY_SET_OUT_INT( F, OP, LT, int8_t ) break; \ case GAL_TYPE_UINT16: BINARY_SET_OUT_INT( F, OP, LT, uint16_t ) break; \ case GAL_TYPE_INT16: BINARY_SET_OUT_INT( F, OP, LT, int16_t ) break; \ case GAL_TYPE_UINT32: BINARY_SET_OUT_INT( F, OP, LT, uint32_t ) break; \ case GAL_TYPE_INT32: BINARY_SET_OUT_INT( F, OP, LT, int32_t ) break; \ case GAL_TYPE_UINT64: BINARY_SET_OUT_INT( F, OP, LT, uint64_t ) break; \ case GAL_TYPE_INT64: BINARY_SET_OUT_INT( F, OP, LT, int64_t ) break; \ default: \ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " \ "address the problem. %d is not a usable type code", \ "BINARY_SET_RT", PACKAGE_BUGREPORT, r->type); \ } /* Set the right operator type. */ #define BINARY_SET_RT(F, OP, LT) \ switch(r->type) \ { \ case GAL_TYPE_UINT8: BINARY_SET_OUT( F, OP, LT, uint8_t ) break; \ case GAL_TYPE_INT8: BINARY_SET_OUT( F, OP, LT, int8_t ) break; \ case GAL_TYPE_UINT16: BINARY_SET_OUT( F, OP, LT, uint16_t ) break; \ case GAL_TYPE_INT16: BINARY_SET_OUT( F, OP, LT, int16_t ) break; \ case GAL_TYPE_UINT32: BINARY_SET_OUT( F, OP, LT, uint32_t ) break; \ case GAL_TYPE_INT32: BINARY_SET_OUT( F, OP, LT, int32_t ) break; \ case GAL_TYPE_UINT64: BINARY_SET_OUT( F, OP, LT, uint64_t ) break; \ case GAL_TYPE_INT64: BINARY_SET_OUT( F, OP, LT, int64_t ) break; \ case GAL_TYPE_FLOAT32: BINARY_SET_OUT( F, OP, LT, float ) break; \ case GAL_TYPE_FLOAT64: BINARY_SET_OUT( F, OP, LT, double ) break; \ default: \ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " \ "address the problem. %d is not a usable type code", \ "BINARY_SET_RT", PACKAGE_BUGREPORT, r->type); \ } /* Set the left operator type only for integers (integer operators can't take floating point types). So floating point types must not be in the list of possibilities. */ #define BINARY_SET_LT_INT(F, OP) \ switch(l->type) \ { \ case GAL_TYPE_UINT8: BINARY_SET_RT_INT( F, OP, uint8_t ) break; \ case GAL_TYPE_INT8: BINARY_SET_RT_INT( F, OP, int8_t ) break; \ case GAL_TYPE_UINT16: BINARY_SET_RT_INT( F, OP, uint16_t ) break; \ case GAL_TYPE_INT16: BINARY_SET_RT_INT( F, OP, int16_t ) break; \ case GAL_TYPE_UINT32: BINARY_SET_RT_INT( F, OP, uint32_t ) break; \ case GAL_TYPE_INT32: BINARY_SET_RT_INT( F, OP, int32_t ) break; \ case GAL_TYPE_UINT64: BINARY_SET_RT_INT( F, OP, uint64_t ) break; \ case GAL_TYPE_INT64: BINARY_SET_RT_INT( F, OP, int64_t ) break; \ default: \ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " \ "address the problem. %d is not a usable type code", \ "BINARY_SET_LT_INT", PACKAGE_BUGREPORT, l->type); \ } /* Set the left operator type. */ #define BINARY_SET_LT(F, OP) \ switch(l->type) \ { \ case GAL_TYPE_UINT8: BINARY_SET_RT( F, OP, uint8_t ) break; \ case GAL_TYPE_INT8: BINARY_SET_RT( F, OP, int8_t ) break; \ case GAL_TYPE_UINT16: BINARY_SET_RT( F, OP, uint16_t ) break; \ case GAL_TYPE_INT16: BINARY_SET_RT( F, OP, int16_t ) break; \ case GAL_TYPE_UINT32: BINARY_SET_RT( F, OP, uint32_t ) break; \ case GAL_TYPE_INT32: BINARY_SET_RT( F, OP, int32_t ) break; \ case GAL_TYPE_UINT64: BINARY_SET_RT( F, OP, uint64_t ) break; \ case GAL_TYPE_INT64: BINARY_SET_RT( F, OP, int64_t ) break; \ case GAL_TYPE_FLOAT32: BINARY_SET_RT( F, OP, float ) break; \ case GAL_TYPE_FLOAT64: BINARY_SET_RT( F, OP, double ) break; \ default: \ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " \ "address the problem. %d is not a usable type code", \ "BINARY_SET_LT", PACKAGE_BUGREPORT, l->type); \ } #endif gnuastro-0.5/lib/gnuastro-internal/arithmetic-and.h0000644000175000017500000000213113215601241017415 00000000000000/********************************************************************* Arithmetic operations on data structures. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __ARITHMETIC_AND_H__ #define __ARITHMETIC_AND_H__ void arithmetic_and(gal_data_t *l, gal_data_t *r, gal_data_t *o); #endif gnuastro-0.5/lib/gnuastro-internal/README0000644000175000017500000000071513121462410015240 00000000000000GNU Astronomy Utilities internal header files --------------------------------------------- The `.h' files in this directory are headers to Gnuastro's internal libraries: libraries that are only available to Gnuastro's programs. These are functions that are mainly to do with running a program, for example the common options to all the programs, functions to manage options and configuration files, timing and etc (the names are hopefully descriptive enough).gnuastro-0.5/lib/gnuastro/0000755000175000017500000000000013217220466012634 500000000000000gnuastro-0.5/lib/gnuastro/README0000644000175000017500000000127312774162326013446 00000000000000GNU Astronomy Utilities library header files ============================================ This directory contins Gnuastro's installed library header files. Once installed, these headers will be installed in the specified '$(prefix)/include/gnuastro' directory (the value of '$(prefix)' can be set at configure time, see the "Installation directory" of the Gnuastro book for more). Inside of Gnuastro, the directory is given the same name to make Gnuastro's internal code similar to what a user would use in their own programs once the header files are installed. The headers that are not installed are kept in the parent directory of this directory mixed with the actual library `.c' source files.gnuastro-0.5/lib/gnuastro/wcs.h0000644000175000017500000000611513174213260013520 00000000000000/********************************************************************* Functions to that only use WCSLIB's functions, not related to FITS. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_WCS_H__ #define __GAL_WCS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /************************************************************* *********** Read WCS *********** *************************************************************/ struct wcsprm * gal_wcs_read_fitsptr(fitsfile *fptr, size_t hstartwcs, size_t hendwcs, int *nwcs); struct wcsprm * gal_wcs_read(char *filename, char *hdu, size_t hstartwcs, size_t hendwcs, int *nwcs); /**************************************************************/ /********** Utilities ************/ /**************************************************************/ struct wcsprm * gal_wcs_copy(struct wcsprm *wcs); void gal_wcs_on_tile(gal_data_t *tile); double * gal_wcs_warp_matrix(struct wcsprm *wcs); void gal_wcs_decompose_pc_cdelt(struct wcsprm *wcs); double gal_wcs_angular_distance_deg(double r1, double d1, double r2, double d2); double * gal_wcs_pixel_scale(struct wcsprm *wcs); double gal_wcs_pixel_area_arcsec2(struct wcsprm *wcs); /**************************************************************/ /********** Conversion ************/ /**************************************************************/ gal_data_t * gal_wcs_world_to_img(gal_data_t *coords, struct wcsprm *wcs, int inplace); gal_data_t * gal_wcs_img_to_world(gal_data_t *coords, struct wcsprm *wcs, int inplace); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_WCS_H__ */ gnuastro-0.5/lib/gnuastro/type.h0000644000175000017500000001254413125235120013703 00000000000000/********************************************************************* Type -- Type information and basic operations. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TYPE_H__ #define __GAL_TYPE_H__ #include #include #include /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_CONFIG_SIZEOF_SIZE_T' that we need below) is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files in Gnuastro's source must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro). */ #ifndef IN_GNUASTRO_BUILD #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /************************************************************* ************** Constants *************** *************************************************************/ /* Macros to identify the type of data. */ enum gal_types { GAL_TYPE_INVALID, /* Invalid (=0 by C standard). */ GAL_TYPE_BIT, /* 1 bit */ GAL_TYPE_UINT8, /* 8-bit unsigned integer. */ GAL_TYPE_INT8, /* 8-bit signed integer. */ GAL_TYPE_UINT16, /* 16-bit unsigned integer. */ GAL_TYPE_INT16, /* 16-bit signed integer. */ GAL_TYPE_UINT32, /* 32-bit unsigned integer. */ GAL_TYPE_INT32, /* 32-bit signed integer. */ GAL_TYPE_UINT64, /* 64-bit unsigned integer. */ GAL_TYPE_INT64, /* 64-bit signed integer. */ GAL_TYPE_FLOAT32, /* 32-bit single precision floating point. */ GAL_TYPE_FLOAT64, /* 64-bit double precision floating point. */ GAL_TYPE_COMPLEX32, /* Complex 32-bit floating point. */ GAL_TYPE_COMPLEX64, /* Complex 64-bit floating point. */ GAL_TYPE_STRING, /* String of characters. */ GAL_TYPE_STRLL, /* Linked list of strings. */ }; /* Define system specific types. For example `size_t' is 4 and 8 bytes on 32 and 64 bit systems respectively. In both cases, the standard defines `size_t' to be unsigned. A similar case exists for `long', but it is signed. During `./configure' the sizeof `size_t' and `long' were found and are used to define an alias for these system specific types. Note: we are not using `else'. This is done because by any chance, if the length of these types is not what is expected (4 or 8), then the aliases are not defined and the compiler will crash. */ #if GAL_CONFIG_SIZEOF_SIZE_T == 4 #define GAL_TYPE_SIZE_T GAL_TYPE_UINT32 #elif GAL_CONFIG_SIZEOF_SIZE_T == 8 #define GAL_TYPE_SIZE_T GAL_TYPE_UINT64 #endif #if GAL_CONFIG_SIZEOF_LONG == 4 #define GAL_TYPE_LONG GAL_TYPE_INT32 #elif GAL_CONFIG_SIZEOF_LONG == 8 #define GAL_TYPE_LONG GAL_TYPE_INT64 #endif /************************************************************* ************** General info *************** *************************************************************/ size_t gal_type_sizeof(uint8_t type); char * gal_type_name(uint8_t type, int long_name); uint8_t gal_type_from_name(char *str); void gal_type_min(uint8_t type, void *in); void gal_type_max(uint8_t type, void *in); int gal_type_is_list(uint8_t type); int gal_type_out(int first_type, int second_type); /************************************************************* ************** To/from string *************** *************************************************************/ char * gal_type_bit_string(void *in, size_t size); char * gal_type_to_string(void *ptr, uint8_t type, int quote_if_str_has_space); int gal_type_from_string(void **out, char *string, uint8_t type); void * gal_type_string_to_number(char *string, uint8_t *type); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TYPE_H__ */ gnuastro-0.5/lib/gnuastro/txt.h0000644000175000017500000000454413175442274013561 00000000000000/********************************************************************* txt -- functions to deal with plain text files. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TXT_H__ #define __GAL_TXT_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Macros.*/ #define GAL_TXT_DELIMITERS " ,\t\f\v" #define GAL_TXT_MAX_FMT_LENGTH 20 /* Status of a line: */ enum gal_txt_line_status_enums { GAL_TXT_LINESTAT_INVALID, GAL_TXT_LINESTAT_BLANK, GAL_TXT_LINESTAT_COMMENT, GAL_TXT_LINESTAT_DATAROW, }; /* Functions */ int gal_txt_line_stat(char *line); gal_data_t * gal_txt_table_info(char *filename, size_t *numcols, size_t *numrows); gal_data_t * gal_txt_table_read(char *filename, size_t numrows, gal_data_t *colinfo, gal_list_sizet_t *indexll, size_t minmapsize); gal_data_t * gal_txt_image_read(char *filename, size_t minmapsize); void gal_txt_write(gal_data_t *input, gal_list_str_t *comment, char *filename); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TXT_H__ */ gnuastro-0.5/lib/gnuastro/tile.h0000644000175000017500000005677013156610402013674 00000000000000/********************************************************************* tile -- work with tesselations over a host dataset. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TILE_H__ #define __GAL_TILE_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /***********************************************************************/ /************** Single tile ******************/ /***********************************************************************/ void gal_tile_start_coord(gal_data_t *tile, size_t *start_coord); void gal_tile_start_end_coord(gal_data_t *tile, size_t *start_end, int rel_block); void * gal_tile_start_end_ind_inclusive(gal_data_t *tile, gal_data_t *work, size_t *start_end_inc); /***********************************************************************/ /************** Series of tiles ******************/ /***********************************************************************/ gal_data_t * gal_tile_series_from_minmax(gal_data_t *block, size_t *minmax, size_t number); /***********************************************************************/ /************** Allocated block **********************/ /***********************************************************************/ gal_data_t * gal_tile_block(gal_data_t *tile); size_t gal_tile_block_increment(gal_data_t *block, size_t *tsize, size_t num_increment, size_t *coord); gal_data_t * gal_tile_block_write_const_value(gal_data_t *tilevalues, gal_data_t *tilesll, int withblank, int initialize); gal_data_t * gal_tile_block_check_tiles(gal_data_t *tiles); void * gal_tile_block_relative_to_other(gal_data_t *tile, gal_data_t *other); void gal_tile_block_blank_flag(gal_data_t *tile_ll, size_t numthreads); /***********************************************************************/ /************** Tile full dataset ********************/ /***********************************************************************/ struct gal_tile_two_layer_params { /* Inputs */ size_t *tilesize; /* Tile size along each dim. (C order). */ size_t *numchannels; /* Channel no. along each dim. (C order). */ float remainderfrac; /* Frac. of remainers in each dim to cut. */ uint8_t workoverch; /* Convolve over channel borders. */ uint8_t checktiles; /* Tile IDs in an img, the size of input. */ uint8_t oneelempertile; /* Only use one element for each tile. */ /* Internal parameters. */ size_t ndim; /* The number of dimensions. */ size_t tottiles; /* Total number of tiles in all dim. */ size_t tottilesinch; /* Number of tiles in one channel. */ size_t totchannels; /* Total number of channels in all dim. */ size_t *channelsize; /* Size of channels along each dimension. */ size_t *numtiles; /* Tile no. in each dim. over-all. */ size_t *numtilesinch; /* Tile no. in each dim. on one channel. */ char *tilecheckname; /* Name of file to check tiles. */ size_t *permutation; /* Tile pos. in memory --> pos. overall. */ size_t *firsttsize; /* See `gal_tile_full_regular_first'. */ /* Actual tile and channel data structures. */ gal_data_t *tiles; /* Tiles array (also linked with `next'). */ gal_data_t *channels; /* Channels array (linked with `next'). */ }; size_t * gal_tile_full(gal_data_t *input, size_t *regular, float remainderfrac, gal_data_t **out, size_t multiple, size_t **firsttsize); void gal_tile_full_sanity_check(char *filename, char *hdu, gal_data_t *input, struct gal_tile_two_layer_params *tl); void gal_tile_full_two_layers(gal_data_t *input, struct gal_tile_two_layer_params *tl); void gal_tile_full_permutation(struct gal_tile_two_layer_params *tl); void gal_tile_full_values_write(gal_data_t *tilevalues, struct gal_tile_two_layer_params *tl, int withblank, char *filename, gal_fits_list_key_t *keys, char *program_string); gal_data_t * gal_tile_full_values_smooth(gal_data_t *tilevalues, struct gal_tile_two_layer_params *tl, size_t width, size_t numthreads); size_t gal_tile_full_id_from_coord(struct gal_tile_two_layer_params *tl, size_t *coord); void gal_tile_full_blank_flag(gal_data_t *tile_ll, size_t numthreads); void gal_tile_full_free_contents(struct gal_tile_two_layer_params *tl); /***********************************************************************/ /************** Function-like macros ******************/ /***********************************************************************/ /* Useful when the input and other types are already known. We want this to be self-sufficient (and be possible to call it independent of `GAL_TILE_PARSE_OPERATE'), so some variables (basic definitions) that are already defined in `GAL_TILE_PARSE_OPERATE' re-defined here. */ #define GAL_TILE_PO_OISET(IT, OT, IN, OTHER, PARSE_OTHER, CHECK_BLANK, OP) { \ IT *i=IN->array; \ gal_data_t *tpo_other=OTHER; /* `OTHER' may be NULL. */ \ gal_data_t *tpo_oblock = OTHER ? gal_tile_block(OTHER) : NULL; \ \ size_t tpo_s_e_i_junk[2]={0,0}; \ IT b, *tpo_st=NULL, *tpo_f=i+IN->size; \ size_t tpo_i_increment=0, tpo_num_i_inc=1; \ size_t tpo_o_increment=0, tpo_num_o_inc=1; \ int tpo_parse_other=(OTHER && PARSE_OTHER); \ gal_data_t *tpo_iblock = gal_tile_block(IN); \ OT *tpo_ost=NULL, *o = tpo_other ? tpo_other->array : NULL; \ int tpo_hasblank = CHECK_BLANK ? gal_blank_present(IN, 0) : 0; \ size_t tpo_s_e_i[2]={0,tpo_iblock->size-1}; /* -1: this is INCLUSIVE */ \ \ \ /* A small sanity check: if `OTHER' is given, and it is a block, */ \ /* then it must have the same size as `IN's block. On the other */ \ /* hand, when `OTHER' is a tile, its must have `IN's size. */ \ if( tpo_parse_other ) \ { \ if( OTHER==tpo_oblock ) /* `OTHER' is a block. */ \ { \ if(gal_data_dsize_is_different(tpo_iblock, tpo_oblock) ) \ { \ /* `error' function, is a GNU extension, see above. */ \ fprintf(stderr, "GAL_TILE_PO_OISET: when " \ "`PARSE_OTHER' is non-zero, the allocated " \ "block size of `IN' and `OTHER' must be " \ "equal, but they are not: %zu and %zu " \ "elements respectively\n", tpo_iblock->size, \ tpo_oblock->size); \ exit(EXIT_FAILURE); \ } \ } \ else \ if(gal_data_dsize_is_different(IN, OTHER) ) \ { \ /* The `error' function, is a GNU extension and this */ \ /* is a header, not a library which the user has to */ \ /* compile every time (on their own system). */ \ fprintf(stderr, "GAL_TILE_PO_OISET: when " \ "`PARSE_OTHER' is non-zero, the sizes of `IN' " \ "and `OTHER' must be equal (in all " \ "dimensions), but they are not: %zu and %zu " \ "elements respectively\n", IN->size, \ tpo_other->size); \ exit(EXIT_FAILURE); \ } \ } \ \ \ /* Write the blank value for the input type into `b'. */ \ gal_blank_write(&b, tpo_iblock->type); \ \ \ /* If this is a tile, not a full block, then we need to set the */ \ /* starting pointers (`tpo_st' and `tpo_ost'). The latter needs */ \ /* special attention: if it is a block, then we will use the */ \ /* the same starting element as the input tile. If `OTHER' is a */ \ /* tile, then use its own starting position (recall that we have */ \ /* already made sure that `IN' and `OTHER' have the same size. */ \ if(IN!=tpo_iblock) \ { \ tpo_st = gal_tile_start_end_ind_inclusive(IN, tpo_iblock, \ tpo_s_e_i); \ if( tpo_parse_other ) \ tpo_ost = ( OTHER==tpo_oblock \ ? ( (OT *)(tpo_oblock->array) \ + ( tpo_st - (IT *)(tpo_iblock->array) ) ) \ : gal_tile_start_end_ind_inclusive(tpo_other, \ tpo_oblock, \ tpo_s_e_i_junk) ); \ } \ \ \ /* Go over contiguous patches of memory. */ \ while( tpo_s_e_i[0] + tpo_i_increment <= tpo_s_e_i[1] ) \ { \ /* If we are on a tile, reset `i' and `o'. */ \ if(IN!=tpo_iblock) \ { \ tpo_f = ( ( i = tpo_st + tpo_i_increment ) \ + IN->dsize[IN->ndim-1] ); \ if(tpo_parse_other) o = tpo_ost + tpo_o_increment; \ } \ \ /* Do the operation depending the nature of the blank value. */ \ /* Recall that for integer types, the blank value must be */ \ /* checked with `=='. But for floats, the blank value can be */ \ /* a NaN. Recall that a NAN will fail any comparison */ \ /* including `=='. So when the blank value is not equal to */ \ /* itself, then it is floating point and is a NAN. In that */ \ /* case, the only way to check if a data element is blank or */ \ /* not is to see if the value of each element is equal to */ \ /* itself or not. */ \ if(tpo_hasblank) \ { \ if(b==b) \ do{if(*i!=b) {OP;} if(tpo_parse_other) ++o;} while(++isize \ : gal_tile_block_increment(tpo_iblock, \ IN->dsize, \ tpo_num_i_inc++, \ NULL) ); \ \ /* Similarly, increment the other array if necessary. Like */ \ /* the above, when `OTHER' is a full block, we'll just use */ \ /* the same increment as `IN'. Otherwise, when `OTHER' is a */ \ /* tile, calculate its increment based on its own block. */ \ if(tpo_parse_other) \ { \ if(OTHER==tpo_oblock) tpo_o_increment=tpo_i_increment; \ else \ tpo_o_increment += gal_tile_block_increment(tpo_oblock, \ tpo_other->dsize, \ tpo_num_o_inc++, \ NULL); \ } \ } \ \ /* This is done in case the caller doesn't need `o' to avoid */ \ /* compiler warnings. */ \ o = o ? o+0 : NULL; \ } #define GAL_TILE_PO_OSET(OT, IN, OTHER, PARSE_OTHER, CHECK_BLANK, OP) { \ switch(tpo_iblock->type) \ { \ case GAL_TYPE_UINT8: \ GAL_TILE_PO_OISET(uint8_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT8: \ GAL_TILE_PO_OISET(int8_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_UINT16: \ GAL_TILE_PO_OISET(uint16_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT16: \ GAL_TILE_PO_OISET(int16_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_UINT32: \ GAL_TILE_PO_OISET(uint32_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT32: \ GAL_TILE_PO_OISET(int32_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_UINT64: \ GAL_TILE_PO_OISET(uint64_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT64: \ GAL_TILE_PO_OISET(int64_t, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_FLOAT32: \ GAL_TILE_PO_OISET(float, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_FLOAT64: \ GAL_TILE_PO_OISET(double, OT,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ default: \ { /* `error' function might not be available for the user. */ \ fprintf(stderr, "GAL_TILE_PO_OSET: type code %d not recognized",\ tpo_iblock->type); \ exit(EXIT_FAILURE); \ } \ } \ } /* Parse over a region of memory (can be an n-dimensional tile or a fully allocated block of memory) and do a certain operation. If `OTHER' is not NULL, this macro will also parse it at the same time . Note that OTHER must either have only one element (for the whole input) or have exactly the same number of elements as the input (one value for one pixel/element of the input). See the documentation for more on this macro and some examples. */ #define GAL_TILE_PARSE_OPERATE(IN, OTHER, PARSE_OTHER, CHECK_BLANK, OP) { \ gal_data_t *tpo_iblock = gal_tile_block(IN); \ gal_data_t *tpo_oblock = OTHER ? gal_tile_block(OTHER) : NULL; \ \ /* First set the OTHER type. */ \ if(OTHER) \ switch(tpo_oblock->type) \ { \ case GAL_TYPE_UINT8: \ GAL_TILE_PO_OSET(uint8_t, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT8: \ GAL_TILE_PO_OSET(int8_t, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_UINT16: \ GAL_TILE_PO_OSET(uint16_t,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT16: \ GAL_TILE_PO_OSET(int16_t, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_UINT32: \ GAL_TILE_PO_OSET(uint32_t,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT32: \ GAL_TILE_PO_OSET(int32_t, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_UINT64: \ GAL_TILE_PO_OSET(uint64_t,IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_INT64: \ GAL_TILE_PO_OSET(int64_t, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_FLOAT32: \ GAL_TILE_PO_OSET(float, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ case GAL_TYPE_FLOAT64: \ GAL_TILE_PO_OSET(double, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ break; \ default: \ { \ fprintf(stderr, "type code %d not recognized in " \ "`GAL_TILE_PARSE_OPERATE'", tpo_oblock->type); \ exit(EXIT_FAILURE); \ } \ } \ else \ /* When `OTHER==NULL', its type is irrelevant, we'll just use */ \ /*`int' as a place holder. */ \ GAL_TILE_PO_OSET(int, IN,OTHER,PARSE_OTHER,CHECK_BLANK,OP); \ } __END_C_DECLS /* From C++ preparations */ #endif gnuastro-0.5/lib/gnuastro/threads.h0000644000175000017500000001043713121462410014353 00000000000000/********************************************************************* Functions to facilitate using threads. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_THREADS_H__ #define __GAL_THREADS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_CONFIG_HAVE_PTHREAD_BARRIER' that we need below) is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro).*/ #ifndef IN_GNUASTRO_BUILD #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /*****************************************************************/ /********* Implementation of pthread_barrier ***************/ /*****************************************************************/ #if GAL_CONFIG_HAVE_PTHREAD_BARRIER == 0 /* Integer number of nano-seconds that `pthread_barrier_destroy' should wait for a check to see if all barriers have been reached. */ #define GAL_THREADS_BARRIER_DESTROY_NANOSECS 1000 typedef int pthread_barrierattr_t; typedef struct { pthread_mutex_t mutex; pthread_cond_t cond; size_t count; size_t limit; size_t condfinished; } pthread_barrier_t; int pthread_barrier_init(pthread_barrier_t *b, pthread_barrierattr_t *attr, unsigned int limit); int pthread_barrier_wait(pthread_barrier_t *b); int pthread_barrier_destroy(pthread_barrier_t *b); #endif /* GAL_CONFIG_HAVE_PTHREAD_BARRIER == 0 */ /*******************************************************************/ /************ Thread utilities **************/ /*******************************************************************/ size_t gal_threads_number(); void gal_threads_dist_in_threads(size_t numactions, size_t numthreads, size_t **outthrds, size_t *outthrdcols); void gal_threads_attr_barrier_init(pthread_attr_t *attr, pthread_barrier_t *b, size_t limit); /*******************************************************************/ /************ Run a function on multiple threads **************/ /*******************************************************************/ struct gal_threads_params { size_t id; /* Id of this thread. */ void *params; /* Input structure for higher-level settings. */ size_t *indexs; /* Indexes of actions to be done in this thread. */ pthread_barrier_t *b; /* Pointer the barrier for all threads. */ }; void gal_threads_spin_off(void *(*worker)(void *), void *caller_params, size_t numactions, size_t numthreads); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_THREADS_H__ */ gnuastro-0.5/lib/gnuastro/table.h0000644000175000017500000001257613211616535014027 00000000000000/********************************************************************* table -- functions for table input and output. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_TABLE_H__ #define __GAL_TABLE_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* `printf' default formattings. Note that the string type shouldn't have any precision and for the width, */ #define GAL_TABLE_DEF_WIDTH_STR 6 #define GAL_TABLE_DEF_WIDTH_INT 6 #define GAL_TABLE_DEF_WIDTH_LINT 10 #define GAL_TABLE_DEF_WIDTH_FLT 13 #define GAL_TABLE_DEF_WIDTH_DBL 18 #define GAL_TABLE_DEF_PRECISION_INT 0 #define GAL_TABLE_DEF_PRECISION_FLT 6 #define GAL_TABLE_DEF_PRECISION_DBL 14 /* Particular display formats for different types: Integers or floating point numbers can be printed in various display formats. The values here are stored in `gal_data_t' when necessary to help in printing of the data.*/ enum gal_table_diplay_formats { GAL_TABLE_DISPLAY_FMT_INVALID, /* Invalid (=0 by C standard). */ GAL_TABLE_DISPLAY_FMT_STRING, /* String/Character. */ GAL_TABLE_DISPLAY_FMT_DECIMAL, /* Integers: signed decimal. */ GAL_TABLE_DISPLAY_FMT_UDECIMAL, /* Integers: unsigned decimal. */ GAL_TABLE_DISPLAY_FMT_OCTAL, /* Integers: octal. */ GAL_TABLE_DISPLAY_FMT_HEX, /* Integers: hexadecimal. */ GAL_TABLE_DISPLAY_FMT_FLOAT, /* Floats: with decimal point. */ GAL_TABLE_DISPLAY_FMT_EXP, /* Floats: as exponential. */ GAL_TABLE_DISPLAY_FMT_GENERAL, /* Floats: general (%g in C). */ }; /* Formats of table storage for input or output, as strings and integers. */ enum gal_table_types { GAL_TABLE_FORMAT_INVALID, /* Invalid (=0 by C standard). */ GAL_TABLE_FORMAT_TXT, /* Plain text table. */ GAL_TABLE_FORMAT_AFITS, /* FITS ASCII table. */ GAL_TABLE_FORMAT_BFITS, /* FITS binary table. */ }; /* When the desired column is not a number, should the string match or regular expression search be in the name, units or comments of the columns? */ enum gal_table_where_to_search { GAL_TABLE_SEARCH_INVALID, /* Invalid (=0 by C standard). */ GAL_TABLE_SEARCH_NAME, /* Match/search in names. */ GAL_TABLE_SEARCH_UNIT, /* Match/search in units. */ GAL_TABLE_SEARCH_COMMENT, /* Match/search in comments. */ }; /************************************************************************/ /*************** Information about a table ***************/ /************************************************************************/ gal_data_t * gal_table_info(char *filename, char *hdu, size_t *numcols, size_t *numrows, int *tableformat); void gal_table_print_info(gal_data_t *allcols, size_t numcols, size_t numrows); /************************************************************************/ /*************** Read a table ***************/ /************************************************************************/ gal_data_t * gal_table_read(char *filename, char *hdu, gal_list_str_t *cols, int searchin, int ignorecase, int minmapsize, size_t *colmatch); /************************************************************************/ /*************** Write a table ***************/ /************************************************************************/ void gal_table_comments_add_intro(gal_list_str_t **comments, char *program_string, time_t *rawtime); void gal_table_write(gal_data_t *cols, gal_list_str_t *comments, int tableformat, char *filename, char *extname); void gal_table_write_log(gal_data_t *logll, char *program_string, time_t *rawtime, gal_list_str_t *comments, char *filename, int quiet); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TABLE_H__ */ gnuastro-0.5/lib/gnuastro/statistics.h0000644000175000017500000001250313121462410015107 00000000000000/********************************************************************* Statistical functions. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_STATISTICS_H__ #define __GAL_STATISTICS_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Maximum number of tests for sigma-clipping convergence. */ #define GAL_STATISTICS_SIG_CLIP_MAX_CONVERGE 50 /* Least acceptable mode symmetricity.*/ #define GAL_STATISTICS_MODE_GOOD_SYM 0.2f /* Enumerators */ enum is_sorted_outputs { GAL_STATISTICS_SORTED_NOT, /* ==0 by C standard. */ GAL_STATISTICS_SORTED_INCREASING, GAL_STATISTICS_SORTED_DECREASING, }; enum bin_status { GAL_STATISTICS_BINS_INVALID, /* ==0 by C standard. */ GAL_STATISTICS_BINS_REGULAR, GAL_STATISTICS_BINS_IRREGULAR, }; /**************************************************************** ******** Simple statistics ******* ****************************************************************/ gal_data_t * gal_statistics_number(gal_data_t *input); gal_data_t * gal_statistics_minimum(gal_data_t *input); gal_data_t * gal_statistics_maximum(gal_data_t *input); gal_data_t * gal_statistics_sum(gal_data_t *input); gal_data_t * gal_statistics_mean(gal_data_t *input); gal_data_t * gal_statistics_std(gal_data_t *input); gal_data_t * gal_statistics_mean_std(gal_data_t *input); gal_data_t * gal_statistics_median(gal_data_t *input, int inplace); size_t gal_statistics_quantile_index(size_t size, double quantile); gal_data_t * gal_statistics_quantile(gal_data_t *input, double quantile, int inplace); size_t gal_statistics_quantile_function_index(gal_data_t *input, gal_data_t *value, int inplace); gal_data_t * gal_statistics_quantile_function(gal_data_t *input, gal_data_t *value, int inplace); /**************************************************************** ******** Mode ******* ****************************************************************/ gal_data_t * gal_statistics_mode(gal_data_t *input, float errorstd, int inplace); gal_data_t * gal_statistics_mode_mirror_plots(gal_data_t *input, gal_data_t *value, size_t numbins, int inplace, double *mirror_val); /**************************************************************** ******** Sort ******* ****************************************************************/ int gal_statistics_is_sorted(gal_data_t *input); void gal_statistics_sort_increasing(gal_data_t *input); void gal_statistics_sort_decreasing(gal_data_t *input); gal_data_t * gal_statistics_no_blank_sorted(gal_data_t *input, int inplace); /**************************************************************** ******** Histogram and Cumulative Frequency Plot ******* ****************************************************************/ gal_data_t * gal_statistics_regular_bins(gal_data_t *data, gal_data_t *range, size_t numbins, double onebinstart); gal_data_t * gal_statistics_histogram(gal_data_t *data, gal_data_t *bins, int normalize, int maxhistone); gal_data_t * gal_statistics_cfp(gal_data_t *data, gal_data_t *bins, int normalize); /**************************************************************** ***************** Sigma clip ******************** ****************************************************************/ gal_data_t * gal_statistics_sigma_clip(gal_data_t *input, float multip, float param, int inplace, int quiet); /****************************************************************/ /************* Identify outliers ****************/ /****************************************************************/ void gal_statistics_remove_outliers_flat_cdf(float *sorted, size_t *outsize); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_STATISTICS_H__ */ gnuastro-0.5/lib/gnuastro/qsort.h0000644000175000017500000000612513121462410014070 00000000000000/********************************************************************* forqsort -- Functions used by qsort to sort an array. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_QSORT_H__ #define __GAL_QSORT_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Pointer used to sort the indexs of an array based on their flux (value in this array). */ extern float *gal_qsort_index_arr; int gal_qsort_index_float_decreasing(const void * a, const void * b); int gal_qsort_uint8_decreasing(const void *a, const void *b); int gal_qsort_uint8_increasing(const void *a, const void *b); int gal_qsort_int8_decreasing(const void *a, const void *b); int gal_qsort_int8_increasing(const void *a, const void *b); int gal_qsort_uint16_decreasing(const void *a, const void *b); int gal_qsort_uint16_increasing(const void *a, const void *b); int gal_qsort_int16_decreasing(const void *a, const void *b); int gal_qsort_int16_increasing(const void *a, const void *b); int gal_qsort_uint32_decreasing(const void *a, const void *b); int gal_qsort_uint32_increasing(const void *a, const void *b); int gal_qsort_int32_decreasing(const void *a, const void *b); int gal_qsort_int32_increasing(const void *a, const void *b); int gal_qsort_uint64_decreasing(const void *a, const void *b); int gal_qsort_uint64_increasing(const void *a, const void *b); int gal_qsort_int64_decreasing(const void *a, const void *b); int gal_qsort_int64_increasing(const void *a, const void *b); int gal_qsort_float32_decreasing(const void *a, const void *b); int gal_qsort_float32_increasing(const void *a, const void *b); int gal_qsort_float64_decreasing(const void *a, const void *b); int gal_qsort_float64_increasing(const void *a, const void *b); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_QSORT_H__ */ gnuastro-0.5/lib/gnuastro/polygon.h0000644000175000017500000000435612772171231014424 00000000000000/********************************************************************* Polygon related functions and macros. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_POLYGON_H__ #define __GAL_POLYGON_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ #define GAL_POLYGON_MAX_CORNERS 50 #define GAL_POLYGON_ROUND_ERR 1e-5 /***************************************************************/ /************** Function declarations ******************/ /***************************************************************/ void gal_polygon_ordered_corners(double *in, size_t n, size_t *ordinds); double gal_polygon_area(double *v, size_t n); int gal_polygon_pin(double *v, double *p, size_t n); int gal_polygon_ppropin(double *v, double *p, size_t n); void gal_polygon_clip(double *s, size_t n, double *c, size_t m, double *o, size_t *numcrn); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_POLYGON_H__ */ gnuastro-0.5/lib/gnuastro/permutation.h0000644000175000017500000000443113121462410015265 00000000000000/********************************************************************* Permutation -- Work on permutations (arrays of indexs). This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_PERMUTATION_H__ #define __GAL_PERMUTATION_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /*********************************************************************/ /*************** Permutation info *******************/ /*********************************************************************/ void gal_permutation_check(size_t *permutation, size_t size); /*********************************************************************/ /*************** Apply permutation *******************/ /*********************************************************************/ void gal_permutation_apply(gal_data_t *input, size_t *permutation); void gal_permutation_apply_inverse(gal_data_t *input, size_t *permutation); __END_C_DECLS /* From C++ preparations */ #endif gnuastro-0.5/lib/gnuastro/match.h0000644000175000017500000000340213211076737014024 00000000000000/********************************************************************* match -- Functions to match catalogs and WCS. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_MATCH_H__ #define __GAL_MATCH_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ gal_data_t * gal_match_coordinates(gal_data_t *coord1, gal_data_t *coord2, double *aperture, int sorted_by_first, int inplace, size_t minmapsize, size_t *nummatched); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_TABLE_H__ */ gnuastro-0.5/lib/gnuastro/list.h0000644000175000017500000001770413121462410013700 00000000000000/********************************************************************* Functions for linked lists. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_LIST_H__ #define __GAL_LIST_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /**************************************************************** ***************** String ******************** ****************************************************************/ typedef struct gal_list_str_t { char *v; struct gal_list_str_t *next; } gal_list_str_t; void gal_list_str_add(gal_list_str_t **list, char *value, int allocate); char * gal_list_str_pop(gal_list_str_t **list); size_t gal_list_str_number(gal_list_str_t *list); void gal_list_str_print(gal_list_str_t *list); void gal_list_str_reverse(gal_list_str_t **list); void gal_list_str_free(gal_list_str_t *list, int freevalue); /**************************************************************** ***************** int32 ******************** ****************************************************************/ typedef struct gal_list_i32_t { int32_t v; struct gal_list_i32_t *next; } gal_list_i32_t; void gal_list_i32_add(gal_list_i32_t **list, int32_t value); int32_t gal_list_i32_pop(gal_list_i32_t **list); size_t gal_list_i32_number(gal_list_i32_t *list); void gal_list_i32_print(gal_list_i32_t *list); void gal_list_i32_reverse(gal_list_i32_t **list); int32_t * gal_list_i32_to_array(gal_list_i32_t *list, int reverse, size_t *num); void gal_list_i32_free(gal_list_i32_t *list); /**************************************************************** ***************** size_t ******************** ****************************************************************/ typedef struct gal_list_sizet_t { size_t v; struct gal_list_sizet_t *next; } gal_list_sizet_t; void gal_list_sizet_add(gal_list_sizet_t **list, size_t value); size_t gal_list_sizet_pop(gal_list_sizet_t **list); size_t gal_list_sizet_number(gal_list_sizet_t *list); void gal_list_sizet_print(gal_list_sizet_t *list); void gal_list_sizet_reverse(gal_list_sizet_t **list); size_t * gal_list_sizet_to_array(gal_list_sizet_t *list, int reverse, size_t *num); void gal_list_sizet_free(gal_list_sizet_t *list); /**************************************************************** ***************** float ******************** ****************************************************************/ typedef struct gal_list_f32_t { float v; struct gal_list_f32_t *next; } gal_list_f32_t; void gal_list_f32_add(gal_list_f32_t **list, float value); float gal_list_f32_pop(gal_list_f32_t **list); size_t gal_list_f32_number(gal_list_f32_t *list); void gal_list_f32_reverse(gal_list_f32_t **list); void gal_list_f32_print(gal_list_f32_t *list); float * gal_list_f32_to_array(gal_list_f32_t *list, int reverse, size_t *num); void gal_list_f32_free(gal_list_f32_t *list); /**************************************************************** ***************** double ******************** ****************************************************************/ typedef struct gal_list_f64_t { double v; struct gal_list_f64_t *next; } gal_list_f64_t; void gal_list_f64_add(gal_list_f64_t **list, double value); double gal_list_f64_pop(gal_list_f64_t **list); size_t gal_list_f64_number(gal_list_f64_t *list); void gal_list_f64_print(gal_list_f64_t *list); void gal_list_f64_reverse(gal_list_f64_t **list); double * gal_list_f64_to_array(gal_list_f64_t *list, int reverse, size_t *num); void gal_list_f64_free(gal_list_f64_t *list); /**************************************************************** ***************** void * ******************** ****************************************************************/ typedef struct gal_list_void_t { void *v; struct gal_list_void_t *next; } gal_list_void_t; void gal_list_void_add(gal_list_void_t **list, void *value); void * gal_list_void_pop(gal_list_void_t **list); size_t gal_list_void_number(gal_list_void_t *list); void gal_list_void_reverse(gal_list_void_t **list); void gal_list_void_free(gal_list_void_t *list, int freevalue); /**************************************************************** ***************** Ordered size_t ******************** ****************************************************************/ typedef struct gal_list_osizet_t { size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_list_osizet_t *next; } gal_list_osizet_t; void gal_list_osizet_add(gal_list_osizet_t **list, size_t value, float tosort); size_t gal_list_osizet_pop(gal_list_osizet_t **list, float *sortvalue); void gal_list_osizet_to_sizet_free(gal_list_osizet_t *in, gal_list_sizet_t **out); /**************************************************************** *********** Doubly linked, ordered size_t ************** ****************************************************************/ typedef struct gal_list_dosizet_t { size_t v; /* The actual value. */ float s; /* The parameter to sort by. */ struct gal_list_dosizet_t *prev; struct gal_list_dosizet_t *next; } gal_list_dosizet_t; void gal_list_dosizet_add(gal_list_dosizet_t **largest, gal_list_dosizet_t **smallest, size_t value, float tosort); size_t gal_list_dosizet_pop_smallest(gal_list_dosizet_t **lartest, gal_list_dosizet_t **smallest, float *tosort); void gal_list_dosizet_print(gal_list_dosizet_t *largest, gal_list_dosizet_t *smallest); void gal_list_dosizet_to_sizet(gal_list_dosizet_t *in, gal_list_sizet_t **out); void gal_list_dosizet_free(gal_list_dosizet_t *largest); /**************************************************************** ***************** gal_data_t ******************** ****************************************************************/ void gal_list_data_add(gal_data_t **list, gal_data_t *newnode); void gal_list_data_add_alloc(gal_data_t **list, void *array, uint8_t type, size_t ndim, size_t *dsize, struct wcsprm *wcs, int clear, size_t minmapsize, char *name, char *unit, char *comment); gal_data_t * gal_list_data_pop(gal_data_t **list); void gal_list_data_reverse(gal_data_t **list); size_t gal_list_data_number(gal_data_t *list); void gal_list_data_free(gal_data_t *list); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_LIST_H__ */ gnuastro-0.5/lib/gnuastro/interpolate.h0000644000175000017500000000367613121462410015256 00000000000000/********************************************************************* tile -- work with tesselations over a host dataset. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_INTERPOLATE_H__ #define __GAL_INTERPOLATE_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ gal_data_t * gal_interpolate_close_neighbors(gal_data_t *input, struct gal_tile_two_layer_params *tl, size_t numneighbors, size_t numthreads, int onlyblank, int aslinkedlist); __END_C_DECLS /* From C++ preparations */ #endif gnuastro-0.5/lib/gnuastro/git.h0000644000175000017500000000322313014150571013502 00000000000000/********************************************************************* Functions to facilitate using the Git library. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_GIT_H__ #define __GAL_GIT_H__ #if GAL_CONFIG_HAVE_LIBGIT2 == 1 #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Only make the Git definitions if the system has LIBGIT2, */ char * gal_git_describe(); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_GIT_H__ */ gnuastro-0.5/lib/gnuastro/fits.h0000644000175000017500000002023313211076737013676 00000000000000/********************************************************************* Functions to convert a FITS array to a C array and vice versa. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_FITS_H__ #define __GAL_FITS_H__ /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_CONFIG_HAVE_WCSLIB_VERION' that we need in `fits.c') is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro).*/ #ifndef IN_GNUASTRO_BUILD #include #endif /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include #include #include #include #include #include #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Macros. */ #define GAL_FITS_MAX_NDIM 999 #define GAL_FITS_KEY_TITLE_START " / " /* To create a linked list of headers. */ typedef struct gal_fits_list_key_t { int kfree; /* ==1, free keyword name. */ int vfree; /* ==1, free keyword value. */ int cfree; /* ==1, free comment. */ uint8_t type; /* Keyword value type. */ char *keyname; /* Keyword Name. */ void *value; /* Keyword value. */ char *comment; /* Keyword comment. */ char *unit; /* Keyword unit. */ struct gal_fits_list_key_t *next; /* Pointer next keyword. */ } gal_fits_list_key_t; /************************************************************* ************** Reporting errors: *************** *************************************************************/ void gal_fits_io_error(int status, char *message); /************************************************************* ************** FITS names *************** *************************************************************/ int gal_fits_name_is_fits(char *name); int gal_fits_suffix_is_fits(char *suffix); char * gal_fits_name_save_as_string(char *filename, char *hdu); /************************************************************* ************** Type codes *************** *************************************************************/ uint8_t gal_fits_bitpix_to_type(int bitpix); int gal_fits_type_to_bitpix(uint8_t type); char gal_fits_type_to_bin_tform(uint8_t type); int gal_fits_type_to_datatype(uint8_t type); uint8_t gal_fits_datatype_to_type(int datatype, int is_table_column); /**************************************************************/ /********** HDU ************/ /**************************************************************/ fitsfile * gal_fits_open_to_write(char *filename); size_t gal_fits_hdu_num(char *filename); int gal_fits_hdu_format(char *filename, char *hdu); fitsfile * gal_fits_hdu_open(char *filename, char *hdu, int iomode); fitsfile * gal_fits_hdu_open_format(char *filename, char *hdu, int img0_tab1); /**************************************************************/ /********** Header keywords ************/ /**************************************************************/ void * gal_fits_key_img_blank(uint8_t type); void gal_fits_key_clean_str_value(char *string); void gal_fits_key_read_from_ptr(fitsfile *fptr, gal_data_t *keysll, int readcomment, int readunit); void gal_fits_key_read(char *filename, char *hdu, gal_data_t *keysll, int readcomment, int readunit); void gal_fits_key_list_add(gal_fits_list_key_t **list, uint8_t type, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit); void gal_fits_key_list_add_end(gal_fits_list_key_t **list, uint8_t type, char *keyname, int kfree, void *value, int vfree, char *comment, int cfree, char *unit); void gal_fits_key_write_filename(char *keynamebase, char *filename, gal_fits_list_key_t **list); void gal_fits_key_write_wcsstr(fitsfile *fptr, char *wcsstr, int nkeyrec); void gal_fits_key_write(fitsfile *fptr, gal_fits_list_key_t **keylist); void gal_fits_key_write_version(fitsfile *fptr, gal_fits_list_key_t *headers, char *program_string); /************************************************************* ****************** Array functions ***************** *************************************************************/ void gal_fits_img_info(fitsfile *fptr, int *type, size_t *ndim, size_t **dsize, char **name, char **unit); gal_data_t * gal_fits_img_read(char *filename, char *hdu, size_t minmapsize, size_t hstartwcs, size_t hendwcs); gal_data_t * gal_fits_img_read_to_type(char *inputname, char *hdu, uint8_t type, size_t minmapsize, size_t hstartwcs, size_t hendwcs); gal_data_t * gal_fits_img_read_kernel(char *filename, char *hdu, size_t minmapsize); fitsfile * gal_fits_img_write_to_ptr(gal_data_t *data, char *filename); void gal_fits_img_write(gal_data_t *data, char *filename, gal_fits_list_key_t *headers, char *program_string); void gal_fits_img_write_to_type(gal_data_t *data, char *filename, gal_fits_list_key_t *headers, char *program_string, int type); void gal_fits_img_write_corr_wcs_str(gal_data_t *input, char *filename, char *wcsheader, int nkeyrec, double *crpix, gal_fits_list_key_t *headers, char *program_string); /**************************************************************/ /********** Table ************/ /**************************************************************/ void gal_fits_tab_size(fitsfile *fitsptr, size_t *nrows, size_t *ncols); int gal_fits_tab_format(fitsfile *fptr); gal_data_t * gal_fits_tab_info(char *filename, char *hdu, size_t *numcols, size_t *numrows, int *tableformat); gal_data_t * gal_fits_tab_read(char *filename, char *hdu, size_t numrows, gal_data_t *colinfo, gal_list_sizet_t *indexll, int minmapsize); void gal_fits_tab_write(gal_data_t *cols, gal_list_str_t *comments, int tableformat, char *filename, char *extname); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_FITS_H__ */ gnuastro-0.5/lib/gnuastro/dimension.h0000644000175000017500000005212613176441456014730 00000000000000/********************************************************************* multidim -- Functions for multi-dimensional operations. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_MULTIDIM_H__ #define __GAL_MULTIDIM_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /************************************************************************/ /******************** Info **********************/ /************************************************************************/ size_t gal_dimension_total_size(size_t ndim, size_t *dsize); size_t * gal_dimension_increment(size_t ndim, size_t *dsize); size_t gal_dimension_num_neighbors(size_t ndim); /************************************************************************/ /******************** Coordinates **********************/ /************************************************************************/ #define GAL_DIMENSION_FLT_TO_INT(FLT) ( (FLT)-(long)(FLT) > 0.5f \ ? (long)(FLT)+1 : (long)(FLT) ) void gal_dimension_add_coords(size_t *c1, size_t *c2, size_t *out, size_t ndim); size_t gal_dimension_coord_to_index(size_t ndim, size_t *dsize, size_t *coord); void gal_dimension_index_to_coord(size_t index, size_t ndim, size_t *dsize, size_t *coord); /************************************************************************/ /******************** Distances **********************/ /************************************************************************/ size_t gal_dimension_dist_manhattan(size_t *a, size_t *b, size_t ndim); /************************************************************************/ /******************** Neighbors **********************/ /************************************************************************/ /* Purpose ------- This macro will allow you to do a fixed operation on the neighbors of an element. The identifier for the element is its dimension-agnostic index (distance from start of array). It is defined as a macro (and not a function) it is often necessary to loop over a very large number of pixels/indexs and the number of neighbors differs (in different dimensions and on the edges of the image). Usage ----- The inputs are: `index': The index of the desired point. `ndim': The number of dimensions in the dataset. `dsize': The size of the dataset along each dimension (C order). `connectivity': The connectivity of the neighbors. This is a single integer with a value between `1' and `ndim' (it is irrelevant for a 1D dataset). Below, the case for 3D data is shown. Each `dn' corresponds to `dinc[n]'. See `dinc' below for the `dinc' values. `1': At most ONE addition/subtraction. In 1D: only the first line should be used. In 2D, this is 4 connectivity. In 3D all the elements that share an 2D-face with the cube at index `i'. i - d0 i + d0 (1D, 2D & 3D) i - d1 i + d1 (2D & 3D) i - d2 i + d2 (3D) `2': At most TWO additions/subtractions. In 2D: 8 connectivity. In 3D: all elements that share a 1D edge with the cube at index `i'. i - d0 - d1 i - d0 + d1 (2D & 3D) i + d0 - d1 i + d0 + d1 (2D & 3D) i - d0 - d2 i - d0 + d2 (3D) i + d0 - d2 i + d0 + d2 (3D) i - d1 - d2 i - d1 + d2 (3D) i + d1 - d2 i + d1 + d2 (3D) `3': At most THREE additions/subtractions (only for 3D and higher dimensions). All cubes that share a 0-D vertex with the cube at index `i'. i - d0 - d1 - d2 i - d0 - d1 + d2 i - d0 + d1 - d2 i - d0 + d1 + d2 i + d0 - d1 - d2 i + d0 - d1 + d2 i + d0 + d1 - d2 i + d0 + d1 + d2 `dinc': An array keeping the length necessary to increment along each dimension. You can make this array with the following function: size_t *dinc=gal_dimension_increment(ndim, dsize); Don't forget to free it afterwards. `operation': Any C operation. `nind' is a `size_t' type variable that is defined by this macro and will have the index of each neighbor. You can use this `nind' for any processing that you like on the neighbor. Note that `op' will be repeated the number of times there is a neighbor. Implementation -------------- To be most efficient (avoid as many `if's as possible), we will start parsing the neighbors from the fastest dimension. When-ever the element is on the edge of the dataset in any dimension, we will store it in a bit-wise array (one bit for each dimension, to mark if it is on the edge (either side 1, or in the middle 0). Far many more elements will be in the middle, so there is no problem to check the edge. The good thing with a bit-array is that it can take one register on the CPU and stay there until the end. But if we want to have an array of values, multiple registers will be necessary. The bit information is in two two-byte spaces, so in theory, this works for 16 dimensions. */ #define GAL_DIMENSION_NEIGHBOR_OP(index, ndim, dsize, connectivity, \ dinc, operation) { \ uint32_t gdn_bitstr=0; \ size_t nind, gdn_ind=index; \ uint8_t gdn_D, *gdn_is_start, *gdn_is_end, *gdn_is_edge, gdn_one=1; \ \ /* A small sanity check. */ \ if(connectivity>ndim) \ error(EXIT_FAILURE, 0, "%s: connectivity value (%d) is larger " \ "than the number of dimensions (%zu)", __func__, \ (int)connectivity, ndim); \ \ /* Initialize the start/end. */ \ gdn_is_start=(uint8_t *)(&gdn_bitstr); \ gdn_is_end=(uint8_t *)(&gdn_bitstr)+1; \ \ /* Start with the slowest dimension and see if it is on the edge */ \ /* or not, similar to `gal_dimension_index_to_coord'. In the */ \ /* process, also fill the `connectivity==1' neighbors. */ \ for(gdn_D=0;gdn_D1 && ndim>1) \ { \ /* Finalize `is_edge' (bit value 1 for respective dim.). */ \ gdn_is_edge=(uint8_t *)(&gdn_bitstr)+2; \ *gdn_is_edge = *gdn_is_start | *gdn_is_end; \ \ /* Shared between 2D and 3D datasets. */ \ if(*gdn_is_edge) \ { /* NOTE: these are bitwise operators, not conditionals. */ \ if( !( *gdn_is_start & ( gdn_one | gdn_one<<1 ) ) ) \ { nind=(index) - (dinc)[0] - (dinc)[1]; {operation;}; } \ if( !( *gdn_is_start & gdn_one ) \ && !( *gdn_is_end & gdn_one<<1 ) ) \ { nind=(index) - (dinc)[0] + (dinc)[1]; {operation;}; } \ if( !( *gdn_is_end & gdn_one ) \ && !( *gdn_is_start & gdn_one<<1 ) ) \ { nind=(index) + (dinc)[0] - (dinc)[1]; {operation;}; } \ if( !( *gdn_is_end & ( gdn_one | gdn_one<<1 ) ) ) \ { nind=(index) + (dinc)[0] + (dinc)[1]; {operation;}; } \ } \ else \ { \ nind=(index) - (dinc)[0] - (dinc)[1]; {operation;}; \ nind=(index) - (dinc)[0] + (dinc)[1]; {operation;}; \ nind=(index) + (dinc)[0] - (dinc)[1]; {operation;}; \ nind=(index) + (dinc)[0] + (dinc)[1]; {operation;}; \ } \ \ /* Only for 3D datasets. */ \ if(ndim>2) \ { \ /* Connectivity == 2. */ \ if(*gdn_is_edge) \ for(gdn_D=0;gdn_D<2;++gdn_D) \ { \ if( !( *gdn_is_start & ( gdn_one<2) \ { \ if(*gdn_is_edge) \ { \ if( !*gdn_is_start ) \ { nind=(index) - (dinc)[0] - (dinc)[1] - (dinc)[2]; \ {operation;}; } \ \ if( !(*gdn_is_start & gdn_one) \ && !(*gdn_is_start & gdn_one<<1) \ && !(*gdn_is_end & gdn_one<<2)) \ { nind=(index) - (dinc)[0] - (dinc)[1] + (dinc)[2]; \ {operation;}; } \ \ if( !(*gdn_is_start & gdn_one) \ && !(*gdn_is_end & gdn_one<<1) \ && !(*gdn_is_start & gdn_one<<2)) \ { nind=(index) - (dinc)[0] + (dinc)[1] - (dinc)[2]; \ {operation;}; } \ \ if( !(*gdn_is_start & gdn_one) \ && !(*gdn_is_end & gdn_one<<1) \ && !(*gdn_is_end & gdn_one<<2)) \ { nind=(index) - (dinc)[0] + (dinc)[1] + (dinc)[2]; \ {operation;}; } \ \ if( !(*gdn_is_end & gdn_one) \ && !(*gdn_is_start & gdn_one<<1) \ && !(*gdn_is_start & gdn_one<<2)) \ { nind=(index) + (dinc)[0] - (dinc)[1] - (dinc)[2]; \ {operation;}; } \ \ if( !(*gdn_is_end & gdn_one) \ && !(*gdn_is_start & gdn_one<<1) \ && !(*gdn_is_end & gdn_one<<2)) \ { nind=(index) + (dinc)[0] - (dinc)[1] + (dinc)[2]; \ {operation;}; } \ \ if( !(*gdn_is_end & gdn_one) \ && !(*gdn_is_end & gdn_one<<1) \ && !(*gdn_is_start & gdn_one<<2)) \ { nind=(index) + (dinc)[0] + (dinc)[1] - (dinc)[2]; \ {operation;}; } \ \ if( !*gdn_is_end ) \ { nind=(index) + (dinc)[0] + (dinc)[1] + (dinc)[2]; \ {operation;}; } \ } \ else \ { \ nind=(index) - (dinc)[0] - (dinc)[1] - (dinc)[2]; \ {operation;}; \ nind=(index) - (dinc)[0] - (dinc)[1] + (dinc)[2]; \ {operation;}; \ nind=(index) - (dinc)[0] + (dinc)[1] - (dinc)[2]; \ {operation;}; \ nind=(index) - (dinc)[0] + (dinc)[1] + (dinc)[2]; \ {operation;}; \ nind=(index) + (dinc)[0] - (dinc)[1] - (dinc)[2]; \ {operation;}; \ nind=(index) + (dinc)[0] - (dinc)[1] + (dinc)[2]; \ {operation;}; \ nind=(index) + (dinc)[0] + (dinc)[1] - (dinc)[2]; \ {operation;}; \ nind=(index) + (dinc)[0] + (dinc)[1] + (dinc)[2]; \ {operation;}; \ } \ } \ } \ } \ \ /* For a check. */ \ /* printf("\nEdge bit flags: "); */ \ /* gal_data_bit_print_stream(&gdn_bitstr, 3); printf("\n"); */ \ } __END_C_DECLS /* From C++ preparations */ #endif gnuastro-0.5/lib/gnuastro/data.h0000644000175000017500000002765213161027175013652 00000000000000/********************************************************************* data -- Structure and functions to represent/work with data This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_DATA_H__ #define __GAL_DATA_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular the `restrict' replacement) is kept in `config.h' (top source directory). When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files in Gnuastro's source must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro). */ #ifndef IN_GNUASTRO_BUILD #include #endif #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Flag values for the dataset. Note that these are bit-values, so to be more clear, we'll use hexadecimal notation: `0x1' (=1), `0x2' (=2), `0x4' (=4), `0x8' (=8), `0x10' (=16), `0x20' (=32) and so on. */ /* Number of bytes in the unsigned integer hosting the bit-flags (`flag' element) of `gal_data_t'. */ #define GAL_DATA_FLAG_SIZE 1 /* Bit 0: The has-blank flag has been checked, so a flag value of 0 for the blank flag is trustable. This can be very useful to avoid repetative checks when the necessary value of the bit is 0. */ #define GAL_DATA_FLAG_BLANK_CH 0x1 /* Bit 1: Dataset contains blank values. */ #define GAL_DATA_FLAG_HASBLANK 0x2 /* Bit 2: Sorted flags have been checked, see GAL_DATA_FLAG_BLANK_CH. */ #define GAL_DATA_FLAG_SORT_CH 0x4 /* Bit 3: Dataset is sorted and increasing. */ #define GAL_DATA_FLAG_SORTED_I 0x8 /* Bit 4: Dataset is sorted and decreasing. */ #define GAL_DATA_FLAG_SORTED_D 0x10 /* Maximum internal flag value. Higher-level flags can be defined with the bitwise shift operators on this value to define internal flags for libraries/programs that depend on Gnuastro without causing any possible conflict with the internal flags or having to check the values manually on every release. */ #define GAL_DATA_FLAG_MAXFLAG GAL_DATA_FLAG_SORTED_D /* Main data structure. mmap (keep data outside of RAM) ------------------------------- `mmap' is C's facility to keep the data on the HDD/SSD instead of inside the RAM. This can be very useful for large data sets which can be very memory intensive. Ofcourse, the speed of operation greatly decreases when defining not using RAM, but that is worth it because increasing RAM might not be possible. So in `gal_data_t' when the size of the requested array (in bytes) is larger than a certain minimum size (in bytes), Gnuastro won't write the array in memory but on non-volatile memory (like HDDs and SSDs) as a file in the `./.gnuastro' directory of the directory it was run from. - If mmapname==NULL, then the array is allocated (using malloc, in the RAM), otherwise its is mmap'd (is actually a file on the ssd/hdd). - minmapsize is stored in the data structure to allow any derivative data structures to follow the same number and decide if they should be mmap'd or allocated. - `minmapsize' == 0: array is definitely mmap'd. - `minmapsize' == -1: array is definitely in RAM. block (work with only a subset of the data) ------------------------------------------- In many contexts, it is desirable to slice the data set into subsets or tiles, not necessarily overlapping. In such a way that you can work on each independently. One option is to copy that region to a separate allocated space, but in many contexts this isn't necessary and infact can be a big burden on CPU/Memory usage. The `block' pointer in `gal_data_t' is defined for situations where allocation is not necessary: you just want to read the data or write to it independently, or in coordination with, other regions of the dataset. Added with parallel processing, this can greatly improve the time/memory consumption. See the figure below for example: assume the larger box is a contiguous block of memory that you are interpretting as a 2D array. But you only want to work on the region marked by the smaller box. tile->block = larger --------------------------- | | | tile | | ---------- | | | | | | |_ | | | |*| | | | ---------- | |_ | |*| | --------------------------- To use `gal_data_t's block concept, you allocate a `gal_data_t *tile' which is initialized with the pointer to the first element in the sub-array (as its `array' argument). Note that this is not necessarily the first element in the larger array. You can set the size of the tile along with the initialization as you please. Recall that, when given a non-NULL pointer as `array', `gal_data_initialize' (and thus `gal_data_alloc') do not allocate any space and just uses the given pointer for the new `array' element of the `gal_data_t'. So your `tile' data structure will not be pointing to a separately allocated space. After the allocation is done, you just point `tile->block' to the `gal_data_t' which hosts the larger array. Afterwards, the programs that take in the `sub' array can check the `block' pointer to see how to deal with dimensions and increments (strides) while working on the `sub' datastructure. For example to increment along the vertical dimension, the program must look at index i+W (where `W' is the width of the larger array, not the tile). Since the block structure is defined as a pointer, arbitrary levels of tesselation/griding are possible. Therefore, just like a linked list, it is important to have the `block' pointer of the largest dataset set to NULL. Normally, you won't have to worry about this, because `gal_data_initialize' (and thus `gal_data_alloc') will set it to NULL by default (just remember not to change it). You can then only change the `block' element for the tiles you define over the allocated space. In Gnuastro, there is a separate library for tiling operations called `tile.h', see the functions there for tools to effectively use this feature. This approach to dealing with parts of a larger block was inspired from the way the GNU Scientific Library does it in the "Vectors and Matrices" chapter. */ typedef struct gal_data_t { /* Basic information on array of data. */ void *restrict array; /* Array keeping data elements. */ uint8_t type; /* Type of data (see `gnuastro/type.h'). */ size_t ndim; /* Number of dimensions in the array. */ size_t *dsize; /* Size of array along each dimension. */ size_t size; /* Total number of data-elements. */ char *mmapname; /* File name of the mmap. */ size_t minmapsize; /* Minimum number of bytes to mmap the array. */ /* WCS information. */ int nwcs; /* for WCSLIB: no. coord. representations. */ struct wcsprm *wcs; /* WCS information for this dataset. */ /* Content descriptions. */ uint8_t flag; /* Flags: currently 8-bits are enough. */ int status; /* Context specific value for the dataset. */ char *name; /* e.g., EXTNAME, or column, or keyword. */ char *unit; /* Units of the data. */ char *comment; /* A more detailed description of the data. */ /* For printing */ int disp_fmt; /* See `gal_table_diplay_formats'. */ int disp_width; /* Width of space to print in ASCII. */ int disp_precision; /* Precision to print in ASCII. */ /* Pointers to other data structures. */ struct gal_data_t *next; /* To use it as a linked list if necessary. */ struct gal_data_t *block; /* `gal_data_t' of hosting block, see above. */ } gal_data_t; /*********************************************************************/ /************* Size and allocation *******************/ /*********************************************************************/ int gal_data_dsize_is_different(gal_data_t *first, gal_data_t *second); void * gal_data_ptr_increment(void *pointer, size_t increment, uint8_t type); size_t gal_data_ptr_dist(void *earlier, void *later, uint8_t type); void * gal_data_malloc_array(uint8_t type, size_t size, const char *funcname, const char *varname); void * gal_data_calloc_array(uint8_t type, size_t size, const char *funcname, const char *varname); void gal_data_initialize(gal_data_t *data, void *array, uint8_t type, size_t ndim, size_t *dsize, struct wcsprm *wcs, int clear, size_t minmapsize, char *name, char *unit, char *comment); gal_data_t * gal_data_alloc(void *array, uint8_t type, size_t ndim, size_t *dsize, struct wcsprm *wcs, int clear, size_t minmapsize, char *name, char *unit, char *comment); void gal_data_free_contents(gal_data_t *data); void gal_data_free(gal_data_t *data); /*********************************************************************/ /************* Array of data structures ******************/ /*********************************************************************/ gal_data_t * gal_data_array_calloc(size_t size); void gal_data_array_free(gal_data_t *dataarr, size_t num, int free_array); /************************************************************* ************** Copying *************** *************************************************************/ gal_data_t * gal_data_copy(gal_data_t *in); gal_data_t * gal_data_copy_to_new_type(gal_data_t *in, uint8_t newtype); gal_data_t * gal_data_copy_to_new_type_free(gal_data_t *in, uint8_t newtype); void gal_data_copy_to_allocated(gal_data_t *in, gal_data_t *out); gal_data_t * gal_data_copy_string_to_number(char *string); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_DATA_H__ */ gnuastro-0.5/lib/gnuastro/cosmology.h0000644000175000017500000000620413173367042014745 00000000000000/********************************************************************* Cosmological calculations. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_COSMOLOGY_H__ #define __GAL_COSMOLOGY_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Age of the universe (in Gyrs). */ double gal_cosmology_age(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Proper distance to z (Mpc). */ double gal_cosmology_proper_distance(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Comoving volume over 4pi stradian to z (Mpc^3). */ double gal_cosmology_comoving_volume(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Critical density at redshift z in units of g/cm^3. */ double gal_cosmology_critical_density(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Angular diameter distance to z (Mpc). */ double gal_cosmology_angular_distance(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Luminosity distance to z (Mpc). */ double gal_cosmology_luminosity_distance(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Distance modulus at z (no units). */ double gal_cosmology_distance_modulus(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); /* Convert apparent to absolute magnitude. */ double gal_cosmology_to_absolute_mag(double z, double H0, double o_lambda_0, double o_matter_0, double o_radiation_0); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_COSMOLOGY_H__ */ gnuastro-0.5/lib/gnuastro/convolve.h0000644000175000017500000000377513136321740014571 00000000000000/********************************************************************* Convolve -- Convolve the dataset with a given kernel. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_CONVOLVE_H__ #define __GAL_CONVOLVE_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ gal_data_t * gal_convolve_spatial(gal_data_t *tiles, gal_data_t *kernel, size_t numthreads, int edgecorrection, int convoverch); void gal_convolve_spatial_correct_ch_edge(gal_data_t *tiles, gal_data_t *kernel, size_t numthreads, int edgecorrection, gal_data_t *tocorrect); __END_C_DECLS /* From C++ preparations */ #endif gnuastro-0.5/lib/gnuastro/box.h0000644000175000017500000000426613216276304013526 00000000000000/********************************************************************* Box -- Define bounding and overlapping boxes. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_BOX_H__ #define __GAL_BOX_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* IMPORTANT NOTE: All the axises are based on the FITS standard, NOT C. */ void gal_box_bound_ellipse_extent(double a, double b, double theta_deg, double *extent); void gal_box_bound_ellipse(double a, double b, double theta_deg, long *width); void gal_box_border_from_center(double *center, size_t ndim, long *width, long *fpixel, long *lpixel); int gal_box_overlap(long *naxes, long *fpixel_i, long *lpixel_i, long *fpixel_o, long *lpixel_o, size_t ndim); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_BOX_H__ */ gnuastro-0.5/lib/gnuastro/blank.h0000644000175000017500000000663013121462410014010 00000000000000/********************************************************************* blank -- Deal with blank values in a datasets This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_BLANK_H__ #define __GAL_BLANK_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_CONFIG_SIZEOF_SIZE_T' that we need below) is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files in Gnuastro's source must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro). */ #ifndef IN_GNUASTRO_BUILD #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Macros: */ /* Blank values: Note that for the unsigned types or small types (like char), the maximum value is considered as a blank value, since the minimum value of an unsigned type is zero and zero is often meaningful in contexts were unsigned values are used. */ #define GAL_BLANK_UINT8 UINT8_MAX #define GAL_BLANK_INT8 INT8_MIN #define GAL_BLANK_UINT16 UINT16_MAX #define GAL_BLANK_INT16 INT16_MIN #define GAL_BLANK_UINT32 UINT32_MAX #define GAL_BLANK_INT32 INT32_MIN #define GAL_BLANK_UINT64 UINT64_MAX #define GAL_BLANK_INT64 INT64_MIN #define GAL_BLANK_FLOAT32 NAN #define GAL_BLANK_FLOAT64 NAN #define GAL_BLANK_STRING "n/a" #if GAL_CONFIG_SIZEOF_SIZE_T == 4 #define GAL_BLANK_SIZE_T GAL_BLANK_UINT32 #else #define GAL_BLANK_SIZE_T GAL_BLANK_UINT64 #endif /* Functions. */ void gal_blank_write(void *pointer, uint8_t type); void * gal_blank_alloc_write(uint8_t type); void gal_blank_initialize(gal_data_t *input); char * gal_blank_as_string(uint8_t type, int width); int gal_blank_present(gal_data_t *input, int updateflag); gal_data_t * gal_blank_flag(gal_data_t *data); void gal_blank_remove(gal_data_t *data); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_DATA_H__ */ gnuastro-0.5/lib/gnuastro/binary.h0000644000175000017500000000717313156610402014214 00000000000000/********************************************************************* binary -- Work on binary (0 and 1 valued) datasets. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_BINARY_H__ #define __GAL_BINARY_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include #include /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* The binary functions will be working on a `uint8_t' type dataset with values of 1 or 0 (no other pixel will be touched). However, in some cases, it is necessary to put temporary values in each element during the processing of the functions. So if your input datasets have values other than 0 and 1 that you don't want these functions to work on, be sure they are not equal to this value. It is chosen as the immediate value before the maximum value for this type (which is the blank value for this type), so blank values will also not be touched by this function. */ #define GAL_BINARY_TMP_VALUE GAL_BLANK_UINT8-1 /*********************************************************************/ /***************** Erosion and dilation ********************/ /*********************************************************************/ gal_data_t * gal_binary_erode(gal_data_t *input, size_t num, int connectivity, int inplace); gal_data_t * gal_binary_dilate(gal_data_t *input, size_t num, int connectivity, int inplace); gal_data_t * gal_binary_open(gal_data_t *input, size_t num, int connectivity, int inplace); /*********************************************************************/ /***************** Connected components ********************/ /*********************************************************************/ size_t gal_binary_connected_components(gal_data_t *binary, gal_data_t **out, int connectivity); gal_data_t * gal_binary_connected_adjacency_matrix(gal_data_t *adjacency, size_t *numnewlabs); /*********************************************************************/ /***************** Fill holes ********************/ /*********************************************************************/ void gal_binary_fill_holes(gal_data_t *input, int connectivity, size_t maxsize); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_DATA_H__ */ gnuastro-0.5/lib/gnuastro/arithmetic.h0000644000175000017500000001377713215601241015065 00000000000000/********************************************************************* Arithmetic -- Preform arithmetic operations on datasets. This is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_ARITHMETIC_H__ #define __GAL_ARITHMETIC_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ #include /* When we are within Gnuastro's building process, `IN_GNUASTRO_BUILD' is defined. In the build process, installation information (in particular `GAL_CONFIG_ARITH_CHAR' and the rest of the types that we needed in the arithmetic function) is kept in `config.h'. When building a user's programs, this information is kept in `gnuastro/config.h'. Note that all `.c' files must start with the inclusion of `config.h' and that `gnuastro/config.h' is only created at installation time (not present during the building of Gnuastro).*/ #ifndef IN_GNUASTRO_BUILD #include #endif /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ /* Arithmetic flags. */ #define GAL_ARITHMETIC_INPLACE 0x1 #define GAL_ARITHMETIC_FREE 0x2 #define GAL_ARITHMETIC_NUMOK 0x4 #define GAL_ARITHMETIC_FLAGS_ALL ( GAL_ARITHMETIC_INPLACE \ | GAL_ARITHMETIC_FREE \ | GAL_ARITHMETIC_NUMOK ) /* Identifiers for each operator. */ enum gal_arithmetic_operators { GAL_ARITHMETIC_OP_INVALID, /* Invalid (=0 by C standard). */ GAL_ARITHMETIC_OP_PLUS, /* + */ GAL_ARITHMETIC_OP_MINUS, /* - */ GAL_ARITHMETIC_OP_MULTIPLY, /* * */ GAL_ARITHMETIC_OP_DIVIDE, /* / */ GAL_ARITHMETIC_OP_MODULO, /* % */ GAL_ARITHMETIC_OP_LT, /* < */ GAL_ARITHMETIC_OP_LE, /* <= */ GAL_ARITHMETIC_OP_GT, /* > */ GAL_ARITHMETIC_OP_GE, /* >= */ GAL_ARITHMETIC_OP_EQ, /* == */ GAL_ARITHMETIC_OP_NE, /* != */ GAL_ARITHMETIC_OP_AND, /* && */ GAL_ARITHMETIC_OP_OR, /* || */ GAL_ARITHMETIC_OP_NOT, /* ! */ GAL_ARITHMETIC_OP_ISBLANK, /* Similar to isnan() for floats. */ GAL_ARITHMETIC_OP_WHERE, /* ?: */ GAL_ARITHMETIC_OP_BITAND, /* & */ GAL_ARITHMETIC_OP_BITOR, /* | */ GAL_ARITHMETIC_OP_BITXOR, /* ^ */ GAL_ARITHMETIC_OP_BITLSH, /* << */ GAL_ARITHMETIC_OP_BITRSH, /* >> */ GAL_ARITHMETIC_OP_BITNOT, /* ~ */ GAL_ARITHMETIC_OP_ABS, /* abs() */ GAL_ARITHMETIC_OP_POW, /* pow() */ GAL_ARITHMETIC_OP_SQRT, /* sqrt() */ GAL_ARITHMETIC_OP_LOG, /* log() */ GAL_ARITHMETIC_OP_LOG10, /* log10() */ GAL_ARITHMETIC_OP_MINVAL, /* Minimum value of array. */ GAL_ARITHMETIC_OP_MAXVAL, /* Maximum value of array. */ GAL_ARITHMETIC_OP_NUMVAL, /* Number of (non-blank) elements. */ GAL_ARITHMETIC_OP_SUMVAL, /* Sum of (non-blank) elements. */ GAL_ARITHMETIC_OP_MEANVAL, /* Mean value of array. */ GAL_ARITHMETIC_OP_STDVAL, /* Standard deviation value of array. */ GAL_ARITHMETIC_OP_MEDIANVAL, /* Median value of array. */ GAL_ARITHMETIC_OP_MIN, /* Minimum per pixel of multiple arrays. */ GAL_ARITHMETIC_OP_MAX, /* Maximum per pixel of multiple arrays. */ GAL_ARITHMETIC_OP_NUM, /* Non-blank number of pixels in arrays. */ GAL_ARITHMETIC_OP_SUM, /* Sum per pixel of multiple arrays. */ GAL_ARITHMETIC_OP_MEAN, /* Mean per pixel of multiple arrays. */ GAL_ARITHMETIC_OP_STD, /* STD per pixel of multiple arrays. */ GAL_ARITHMETIC_OP_MEDIAN, /* Median per pixel of multiple arrays. */ GAL_ARITHMETIC_OP_TO_UINT8, /* Convert to uint8_t. */ GAL_ARITHMETIC_OP_TO_INT8, /* Convert to int8_t. */ GAL_ARITHMETIC_OP_TO_UINT16, /* Convert to uint16_t. */ GAL_ARITHMETIC_OP_TO_INT16, /* Convert to int16_t. */ GAL_ARITHMETIC_OP_TO_UINT32, /* Convert to uint32_t. */ GAL_ARITHMETIC_OP_TO_INT32, /* Convert to int32_t. */ GAL_ARITHMETIC_OP_TO_UINT64, /* Convert to uint64_t. */ GAL_ARITHMETIC_OP_TO_INT64, /* Convert to int64_t. */ GAL_ARITHMETIC_OP_TO_FLOAT32, /* Convert to float32. */ GAL_ARITHMETIC_OP_TO_FLOAT64, /* Convert to float64. */ GAL_ARITHMETIC_OP_LAST_CODE, /* Last code of the library operands. */ }; gal_data_t * gal_arithmetic(int operator, int flags, ...); __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_ARITHMETIC_H__ */ gnuastro-0.5/lib/gnuastro/config.h0000444000175000017500000000523613217220212014163 00000000000000/********************************************************************* Functions dealing with general aspects of all Gnuastro. Original author: Mohammad Akhlaghi Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see . **********************************************************************/ #ifndef __GAL_CONFIG_H__ #define __GAL_CONFIG_H__ /* Include other headers if necessary here. Note that other header files must be included before the C++ preparations below */ /* The restrict keyword might not be present on some systems, so we are redefining it here based on the checks in `configure.ac', see there for more comments. */ #define restrict __restrict /* Configuration macros: */ #define GAL_CONFIG_VERSION "0.5" #define GAL_CONFIG_HAVE_LIBGIT2 1 #define GAL_CONFIG_HAVE_WCSLIB_VERSION 1 #define GAL_CONFIG_HAVE_PTHREAD_BARRIER 1 #define GAL_CONFIG_BIN_OP_UINT8 @HAVE_BIN_OP_UINT8@ #define GAL_CONFIG_BIN_OP_INT8 @HAVE_BIN_OP_INT8@ #define GAL_CONFIG_BIN_OP_UINT16 @HAVE_BIN_OP_UINT16@ #define GAL_CONFIG_BIN_OP_INT16 @HAVE_BIN_OP_INT16@ #define GAL_CONFIG_BIN_OP_UINT32 @HAVE_BIN_OP_UINT32@ #define GAL_CONFIG_BIN_OP_INT32 @HAVE_BIN_OP_INT32@ #define GAL_CONFIG_BIN_OP_UINT64 @HAVE_BIN_OP_UINT64@ #define GAL_CONFIG_BIN_OP_INT64 @HAVE_BIN_OP_INT64@ #define GAL_CONFIG_BIN_OP_FLOAT32 @HAVE_BIN_OP_FLOAT32@ #define GAL_CONFIG_BIN_OP_FLOAT64 @HAVE_BIN_OP_FLOAT64@ #define GAL_CONFIG_SIZEOF_LONG 8 #define GAL_CONFIG_SIZEOF_SIZE_T 8 /* C++ Preparations */ #undef __BEGIN_C_DECLS #undef __END_C_DECLS #ifdef __cplusplus # define __BEGIN_C_DECLS extern "C" { # define __END_C_DECLS } #else # define __BEGIN_C_DECLS /* empty */ # define __END_C_DECLS /* empty */ #endif /* End of C++ preparations */ /* Actual header contants (the above were for the Pre-processor). */ __BEGIN_C_DECLS /* From C++ preparations */ __END_C_DECLS /* From C++ preparations */ #endif /* __GAL_CONFIG_H__ */ gnuastro-0.5/.autom4te.cfg0000644000175000017500000000176012722534072012452 00000000000000# Configuration file for autom4te # =============================== # autom4te is used to create the familiar `./configure' script from # configure.ac (hand written by Gnuastro developers). autom4te is # called during the bootstrapping process (see README-hacking, or the # "Bootstrapping" section in the manual). # # To speed up the process, a directory (`autom4te.cache') is created # which keeps cache information which can speed up its next call. But # this directory is built in the top Gnuastro directory which just # redundantly fills it up with a non-edited directory. So through this # configuration file, we are asking autom4te to make its cache # directory within the bootstrapped directory to keep things on the # top directory clean. # We are using the Autoconf manual's "Customizing autom4te" and # "Invoking autom4te" sections as a reference for this file. begin-language: "Autoconf-without-aclocal-m4" args: --cache=./bootstrapped/autom4te.cache end-language: "Autoconf-without-aclocal-m4"gnuastro-0.5/tmpfs-config-make0000755000175000017500000000665413213252016013404 00000000000000#! /bin/sh # This script will configure and build Gnuastro in parallel within a # temporary tmpfs directory in the RAM. Please see the "Configure and build # in RAM" section of the Gnuastro book/documentation for a full # explanation. # # Original author: Mohammad Akhlaghi # Contributing author(s): # Mosè Giordano # Copyright (C) 2016, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it under # the terms of the GNU General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # Gnuastro is distributed in the hope that it will be useful, but WITHOUT # ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or # FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for # more details. # # You should have received a copy of the GNU General Public License along # with Gnuastro. If not, see . # Set the variables: NUM_THREADS=8 TMPDIR=/dev/shm debug_noshared=0 # Check if TMPDIR exists if [ ! -d $TMPDIR ]; then echo "$TMPDIR doesn't exist. Aborted." exit 1 fi # Keep the address of this source directory (where this script is being run # from) which we will need later. srcdir=$(pwd) # Set the build directory name in tmpfs. If the .version file exists, use # it to allow multiple version builds there (which might happen during # development). basedir=$(basename -- "$srcdir") if [ -f .version ]; then build_dir=$TMPDIR/"$basedir"-$(cat .version) else build_dir=$TMPDIR/"$basedir" fi # Make the build directory in tmpfs (if it doesn't already exist). if [ ! -d $build_dir ]; then mkdir $build_dir fi # Make a symbolic link to the tmpfs build directory for users to easily # access the built files and also follow the progress. We are first # deleting any existing symbolic link and remaking it since the possible # deletion of $build_dir during the development can complicate the # pre-existing symbolic link. build_sym=build if [ -h $build_sym ]; then # Delete a harmless symbolic link, if present. rm $build_sym fi # Create the link only if the symbolic link doesn't exist. if [ ! -e $build_sym ]; then ln -s $build_dir $build_sym else echo "$build_sym already exists here and is not a symbolic link." echo "Aborted." exit 1 fi # Go into the build directory to start the configure and/or build: cd $build_dir # If a 'Makefile' doesn't exist, then configure Gnuastro. # # FOR DEBUGGING: uncomment the second half of this line. Gnuastro uses GNU # Libtool to build shared libraries for highly portable and maintainable # usage on a wide variety of systems. While this is great for binaries, # shared libraries can be a pain when debuggin. For this reason, # compilation of shared libraries can be turned off by specifying the # --disable-shared option to configure. With static libraries, compilation # (the `make' command) will also significantly speed up. Also, by default # (in `configure.ac'), we have set optimization flags which have to be # cancelled in debugging. if [ ! -f Makefile ]; then if [ x$debug_noshared = x1 ]; then $srcdir/configure --srcdir=$srcdir CFLAGS="-g -O0" --disable-shared else $srcdir/configure --srcdir=$srcdir fi fi # Build Gnuastro in that directory with the specified number of threads make -kj$NUM_THREADS gnuastro-0.5/.version0000644000175000017500000000000413217220023011611 000000000000000.5 gnuastro-0.5/.dir-locals.el0000644000175000017500000000151013121462410012561 00000000000000;; This files contains Emacs Directory Local Variables. ;; ;; Emacs is an extensible, customizable, free/libre text editor. It ;; allows specification of certain settings that will be applied to ;; all files in current directory and its subdirectories. This is ;; useful in order to automatically enforce certain coding conventions ;; for all contributors of Gnuastro, like the maximum length of lines ;; or the number of spaces to be used for indentation. ;; ;; For more information see (info "(emacs) Directory Variables") ((nil (indent-tabs-mode . nil) ;; No tabs as indentation (fill-column . 75)) ;; 75-character wide lines (c-mode (c-basic-offset . 2) ;; 2 spaces of indentation (c-file-style . "gnu")) ;; GNU style for braces (makefile-mode (indent-tabs-mode . t)) ;; Real TABs are important in makefiles ) gnuastro-0.5/genauthors0000755000175000017500000000627413121462410012251 00000000000000#! /bin/sh # # Generate a list of authors from the git repository, it will only # actually do anything if a .git file exists. Run like this: # # ./genauthors top/bin/dir # # Note that some authors might have changed their email addresses over # the course of their contributions to Gnuastro. Fortunately Git has a # great tool for that: the .mailmap file. It has already been included # in the source code and if any author changes their email address or # would want their name to be printed differently here, please use # that file. See the git-shortlog manpage for a complete explanation # of all the possible ways to do this. # # Original author: # Mohammad Akhlaghi # Contributing author(s): # Copyright (C) 2015, Free Software Foundation, Inc. # # Gnuastro is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # Gnuastro is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with Gnuastro. If not, see . # Initial settings: set -o nounset # Stop if a variable is not set. set -o errexit # Stop if a program returns false. # Only do the job if a .git directory exists (recall that this script # is also present in the tar-ball with no .git directory and might be # run from there) if [ ! -d "$1/.git" ]; then echo "There is no Git repository in the source directory." echo "AUTHORS cannot be generated." exit 0 fi # Print a status report, since this will be run along with the large # number of bootstrap operations, it is best to tell the users since # it might take a few seconds. echo "Generating AUTHORS from the version controlled source..." # Make sure the .mailmap file is present in this directory, so Git can fix # the different email addresses and names of one person. Note that while # this is in the top source directory, it is possible for the source and # build directories to be different, and we have to be prepared for that. if [ ! -f .mailmap ]; then ln -s $1/.mailmap .mailmap fi # Set the version number. Note that this script is also run at the start of # the bootstrapping process. At that point we don't have the `.version' # file, so we will just rely on `.git describe'. Later during `make', this # scripot will be run again to set it using `git-version-gen'. if [ -f "$1/.version" ]; then gnuastroversion="Gnuastro "$(cat "$1/.version") else gnuastroversion=$(git --git-dir=$1/.git describe) fi # Print the top of the AUTHORS file. echo "GNU Astronomy Utilities (Gnuastro) authors ========================================== Generated for $gnuastroversion. Ordered by number of commits in the Git project history. " > $1/AUTHORS # Generate the aggregate list git --git-dir=$1/.git shortlog --summary --email --no-merges \ --numbered >> $1/AUTHORS gnuastro-0.5/THANKS0000644000175000017500000000637113215601241011056 00000000000000GNU Astronomy Utilities Acknowledgments ======================================= The following people and institutions who contributed to Gnuastro indirectly (not by actually submitting code) are listed here. For the list of Gnuastro code/documentation authors (people who have contributed actual code/text as commits in the version controlled history of Gnuastro), please see the `AUTHORS' file in the same directory. People ------ The following people provided valuable feedback (suggestions, ideas) to the authors of Gnuastro. We hereby gratefully acknowledge their help and support in Gnuastro. The list is ordered alphabetically (by family name). Marjan Akbari mrjakbari@gmail.com Roland Bacon roland.bacon@univ-lyon1.fr Karl Berry karl@gnu.org Leindert Boogaard boogaard@strw.leidenuniv.nl Nicolas Bouché nicolas.bouche@irap.omp.eu Fernando Buitrago fbuitrago@oal.ul.pt Adrian Bunk bunk@debian.org Rosa Calvi rcalvi@iac.es Benjamin Clement benjamin.clement@univ-lyon1.fr Antonio Diaz Diaz antonio@gnu.org Thérèse Godefroy godef.th@free.fr Madusha Gunawardhana gunawardhana@strw.leidenuniv.nl Stephen Hamer stephen.hamer@univ-lyon1.fr Takashi Ichikawa ichikawa@astr.tohoku.ac.jp Raúl Infante Sainz infantesainz@gmail.com Brandon Invergo brandon@gnu.org Aurélien Jarno aurelien.jarno@univ-lyon1.fr Lee Kelvin l.s.kelvin@ljmu.ac.uk Mohammad-Reza Khellat moha.khe@gmail.com Floriane Leclercq floriane.leclercq@univ-lyon1.fr Alan Lefor alefor@astr.tohoku.ac.jp Guillaume Mahler guillaume.mahler@univ-lyon1.fr Francesco Montanari francesco.montanari@openmailbox.org William Pence william.pence@nasa.gov Bob Proulx bob@proulx.com Yahya Sefidbakht y.sefidbakht@gmail.com Alejandro Serrano Borlaff asborlaff@ucm.es Lee Spitler lee.spitler@mq.edu.au Richard Stallman rms@gnu.org Ole Streicher olebole@debian.org Alfred M. Szmidt ams@gnu.org Ignacio Trujillo trujillo@iac.es David Valls-Gabaud david.valls-gabaud@obspm.fr Christopher Willmer cnaw@as.arizona.edu Teams ----- The members of the following teams also provided great help and support. GNU French Translation Team: https://savannah.gnu.org/projects/www-fr Institutions ------------ Host institutions of Gnuastro's developers. Ministry of education, culture, sports, science and technology, Japan. Tohoku University, Sendai, Japan. University of Salento, Lecce, Italy. Centre de Recherche Astrophysique de Lyon, France Centre national de la recherche scientifique, France gnuastro-0.5/NEWS0000644000175000017500000011737213217176176010666 00000000000000GNU Astronomy Utilities NEWS -*- outline -*- * Noteworthy changes in release 0.5 (library 3.0.0) (2017-12-22) [stable] ** New features Manual/Book: An extended tutorial is added showing some general applications of almost all the programs. This may be a good place to get a feeling of how Gnuastro is intended to be used and some of the programs. New Program and library: Match is a new program that will match two given inputs (currently catalogs). Its output is the re-arranged inputs with the same number of rows/records such that all the rows match. The main work is also done with the new low-level `gal_match_catalog' library function which can also be used in more generic contexts. All programs: a value of `0' to the `--numthreads' option will use the number of threads available to the system at run time. Arithmetic: The new operators `filter-median' and `filter-mean' can be used to filter (smooth) the input. The size of the filter can be set as the other operands to these operators. BuildProgram: The new `--la' option allows the identification of a different Libtool `.la' file for Libtool linking information. BuildProgram: The new `--deletecompiled' option will delete the compiled program after running it. CosmicCalculator: all the various cosmological calculations can now be requested individually in one line with a specific option added for each calculation (for example `--age' or `--luminositydist' for the age of the universe at a given redshift or the luminosity distance). Therefore the old `--onlyvolume' and `--onlyabsmagconv' options are now removed. To effectively use these new features, please review the "Invoking CosmicCalculator" section of the book. Fits: when an extension/HDU is identified on the command-line with the `--hdu' option and no operation is requested, the full list of header keywords in that HDU will be printed (as if only `--printallkeys' was called). MakeCatalog: physical nature agnostic WCS column names. Previously the first WCS axis was always assumed to be RA and the second DEC. So for example even if you had a spectrum (with X and wavelength as the two WCS dimensions), you would have to ask for `--ra' and `--dec'. The new `--w1' and `--w2' options are now generic and don't assume any particular type only their order in the FITS header. MakeCatalog now also uses the CTYPE and CUNIT keywords to set the names and units of its output columns. The `--ra' and `--dec' options are now just internal aliases for `--w1' or `--w2' which will be determined based on the input's CTYPE keyword. Also the new `--geow1', `--geow2', `--clumpsw1', `--clumpsw2', `--clumpsgeow1', `--clumpsgeow2' options replace the old options `--geora', `--geodec', `--clumpsra', `--clumpsdec', `--clumpsgeora', `--clumpsgeodec'. No alias is currently defined for the latter group. MakeCatalog: the new `--uprange' option allows you to specify a range for the random values around each object. This is useful when the noise properties of the dataset vary gradually and sampling from the whole dataset might produce biased results. NoiseChisel: with the new `--convolved' and `--convolvedhdu' options, NoiseChisel will not convolve the input any more and use the given dataset instead. In many cases, as the inputs get larger, convolution is the most time consuming step of NoiseChisel. With this option, you can greatly speed up your tests (to find the best parameters by varying them, for a given analysis). See the book for more information and examples. NoiseChisel: with the new `--widekernel' option it is now possible to use a wider kernel to identify which tiles contain signal. The rest of the steps (identifying the quantile threshold on the selected tiles and etc) are done on the dataset convolved with `--kernel' as they were before. Since it is time consuming, this is an optional feature. NoiseChisel: with the new `--qthreshtilequant' option, it is now possible to discard high-valued (outlier) tiles before estimating qthresh over the whole image. This can be useful in detecting very large diffuse/flat regions that would otherwise be detected as background (and effectively removed). NoiseChisel: the finally selected true detections are now grown based on signal contiguity, not by blind dilation. The growth process is the same as the growing of clumps to define objects. Only for true detections, the growth occurs in the noise. You can configure this growth with the `--detgrowquant' and `--detgrowmaxholesize'. With this new feature it is now possible to detect signal out to much lower surface brightness limits and the detections don't look boxy any more. Cosmology library: A new set of cosmology functions are now included in the library (declared in `gnuastro/cosmology.h'). These functions are also used in the CosmicCalculator program. `gal_table_read' can now return the number of columns matched with each input column (for example with regular expressions), a new argument has been added to allow this feature. `gal_fits_key_img_blank': returns the value that must be used in the BLANK keyword for the given type as defined by the FITS standard. `gal_txt_write' and `gal_fits_tab_write' now accept an extension name as argument to allow a name for the FITS extension they write. `gal_box_bound_ellipse_extent' will return the maximum extent of an ellipse along each axis from the ellipse center in floating point. ** Removed features Installation: The `--enable-bin-op-*' configuration options that were introduced in Gnuastro 0.3 have been removed. By managing the arithmetic functions in a better manner (a separate source file for each operator), compilation for all types (when done in parallel) takes about the same time as it took with the default (only four) types until now. MakeCatalog: `--zeropoint' option doesn't have a short option name any more. Previously it was `-z' which was confusing because `-x' and `-y' were used to refer to image coordinate positions. NoiseChisel: The `--dilate' and `--dilatengb' options have been removed. Growing of true detections is no longer done through dilation but through the `--detgrowquant' and `--detgrowmaxholesize' options (see above). ** Changed features CosmicCalculator: The redshift is no longer mandatory. When no redshift is given, it will only print the input parameters (cosmology) and abort. MakeCatalog: when the output is a FITS file, the two object and clumps catalogs will be stored as multiple extensions of a single file. Until now, two separate FITS files would be created. Plain text outputs are the same as before (two files will be created). `gal_binary_fill_holes' now accepts a `connectivity' and `maxsize' argument to specify the connectivity of the holes and the maximum size of acceptable holes to fill. `gal_fits_img_read' and `gal_fits_img_read_to_type' now also read the WCS structure of the extension/HDU in a FITS file and have two extra arguments: `hstartwcs' and `hendwcs'. With these options it is possible to limit the range of header keywords to read the WCS, similar to how they are used in `gal_wcs_read'. `gal_txt_write', `gal_table_write_log', `gal_fits_tab_write' and `gal_txt_write' don't have the `dontdelete' argument any more. The action they take if the file already exists depends on the file: for FITS, a new extension will be added and for text, they will abort with an error. `gal_tile_block_write_const_value' and `gal_tile_full_values_write' now accept a new `withblank' option to set all pixels that are blank in the tile's block to be blank in the check image. `gal_wcs_pixel_area_arcsec2' will return NaN (instead of aborting) when input is unreasonable (not two dimensions or not in units of degrees). `gal_wcs_world_to_img' and `gal_wcs_img_to_world': Until now, these two WCS conversion functions would explicitly assume RA and Dec and work based on input arrays (so for example it was also necessary to give the number of elements and etc). They now accept `gal_data_t' as input for the input coordinates, thus their API has been greatly simplified and their functionality increased. ** Bug fixes ConvertType crash when changing values (bug #52010). Arithmetic not accounting for integer blank pixels in binary operators (bug #52014). NoiseChisel segfault when memory mapping to a file (bug #52043). CFITSIO 3.42 and libcurl crash at Gnuastro configure time (bug #52152). MakeCatalog crash in upper-limit with full size label (bug #52281). NoiseChisel leaving unlabeled regions after clump growth (bug #52327). Arithmetic crash with no input tokens (bug #52422). Libtool checks only in non-current directory (bug #52427). * Noteworthy changes in release 0.4 (library 2.0.0) (2017-09-13) [stable] ** New features All programs: `.fit' is now a recognized FITS file suffix. All programs: ASCII text files (tables) created with CRLF line terminators (for example text files created in MS Windows) are now also readable as input when necessary. Arithmetic: now has a new `--globalhdu' (`-g') option which can be used once for all the input images. MakeNoise: with the new `--sigma' (`-s') option, it is now possible to directly request the noise sigma or standard deviation. When this option is called, the `--background', `--zeropoint' and other option values will be ignored. MakeProfiles: the new `--kernel' option can make a kernel image without the need to define a catalog. With this option, a catalog (or accompanying background image) must not be given. MakeProfiles: the new `--pc', `--cunit' and `--ctype' options can be used to specify the PC matrix, CUNIT and CTYPE world coordinate system keywords of the output FITS file. MakeProfiles: the new `distance' profile will save the radial distance of each pixel. This may be used to define your own profiles that are not currently supported in MakeProfiles. MakeProfiles: with the new `--mcolisbrightness' ("mcol-is-brightness") option, the `--mcol' values of the catalog will be interpretted as total brightness (sum of pixel values), not magnitude. NoiseChisel: with the new `--dilatengb' option, it is now possible to identify the connectivity of the final dilation. Library: Functions that read data from an ASCII text file (`gal_txt_table_info', `gal_txt_table_read', `gal_txt_image_read') now also operate on files with CRLF line terminators. ** Removed features ** Changed features Crop: The new `--center' option is now used to define the center of a single crop. Hence the old `--ra', `--dec', `--xc', `--yc' have been removed. This new option can take multiple values (one value for each dimension). Fractions are also acceptable. Crop: The new `--width' option is now used to define the width of a single crop. Hence the old `--iwidth', `--wwidth' were removed. The units to interpret the value to the option are specified by the `--mode' option. With the new `--width' option it is also possible to define a non-square crop (different widths along each dimension). In WCS mode, its units are no longer arcseconds but are the same units of the WCS (degrees for angles). `--width' can also accept fractions. So to set a width of 5 arcseconds, you can give it a value of `5/3600' for the angular dimensions. Crop: The new `--coordcol' option is now used to determine the catalog columns that define coordinates. Hence the old `--racol', `--deccol', `--xcol', and `--ycol' have been removed. This new option can be called multiple times and the order of its calling will be used for the column containing the center in the respective dimension (in FITS format). MakeNoise: the old `--stdadd' (`-s') option has been renamed to `--instrumental' (`-i') to be more clear. MakeProfiles: The new `--naxis' and `--shift' options can take multiple values for each dimension (separated by a comma). This replaces the old `--naxis1', `--naxis2' and `--xshift' and `--yshift' options. MakeProfiles: The new `--ccol' option can take the center coordinate columns of the catalog (in multiple calls) and the new `--mode' option is used to identify what standard to interpret them in (image or WCS). Together, these replace the old `--xcol', `--ycol', `--racol' and `--deccol'. MakeProfiles: The new `--crpix', `--crval' and `--cdelt' options now accept multiple values separated by a comma. So they replace the old `--crpix1', `--crpix2', `--crval1', `--crval2' and `--resolution' options. `gal_data_free_contents': when the input `gal_data_t' is a tile, its `array' element will not be freed. This enables safe usage of this function (and thus `gal_data_free') on tiles without worrying about the memory block associated with the tile. `gal_box_bound_ellipse' is the new name for the old `gal_box_ellipse_in_box' (to be more clear and avoid repetition of the term `box'). The input position angle is now also in degrees, not radians. `gal_box_overlap' now works on data of any dimensionality and thus also needs the number of dimensions (elements in each input array). `gal_box_border_from_center' now accepts an array of coordinates as one argument and the number of dimensions as another. This allows it to work on any dimensionality. `gal_fits_img_info' now also returns the name and units of the dataset (if they aren't NULL). So it takes two extra arguments. `gal_wcs_pixel_scale' now replaces the old `gal_wcs_pixel_scale_deg', since it doesn't only apply to degrees. The pixel scale units are defined by the units of the WCS. `GAL_TILE_PARSE_OPERATE' (only when `OTHER' is given) can now parse and operate on different datasets independent of the size of allocated block of memory (the tile sizes of `IN' and `OTHER' have to be identical, but not their allocated blocks of memory). Until now, it was necessary for the two blocks to have the same size and this is no longer the case. ** Bug fixes MakeProfiles long options on 32bit big endian systems (bug #51341). Pure rotation around pixel coordinate (0,0) (bug #51353). NoiseChisel segfault when no usable region for sky clumps (bug #51372). Pixel scale measurement when dimension scale isn't equal or doesn't decrease (bug #51385). Improper types for function code in MakeProfiles (bug #51467). Crashes on 32-bit and big-endian systems (bug #51476). Warp's align matrix when second dimension must be reversed (bug #51536). Reading BZERO for unsigned 64-bit integers (bug #51555). Arithmetic with one file and no operators (bug #51559). NoiseChisel segfault when detection contains no clumps (bug #51906). Correct size checking when allocating gal_data_t (bug #52544). * Noteworthy changes in release 0.3 (library 1.0.0) (2017-06-01) [stable] This is a full re-write of Gnuastro. Most importantly, Gnuastro now has a new generic data container (`gal_data_t'). This new container can now deal natively with all standard numeric data types, work in RAM or HDD/SSD, keep data in any dimensions and has enabled many other very useful features. Some of the most prominent of the new features are discussed below. It is strongly recommended to review the respective section of the Gnuastro manual/book for a better feeling of all the new features. As discussed below, some program names have changed, if you have a previous version of Gnuastro installed from source, it is recommended to uninstall it first (with `make uninstall' using the corresponding tarball), then install this new version. Building Gnuastro can be slow, so please build in parallel with Make's `-j8' option (to build on 8 threads). ** New programs or library features Library functions that deal with datasets now use this generic data container for inputs and outputs, significantly simplifying their API. Nearly all library functions have been re-written with much more clear names, argument lists and individual purpose. Some example library functions are shown below, also see the "Library demos" section of the book for some complete working example: -- `gal_table_read' and `gal_table_write' will read and write data to plain text, FITS ASCII and FITS Binary formats. -- `gal_fits_img_read' and `gal_fits_img_write' can read a FITS image to memory or write a FITS image from memory. Gnuastro now defines a simple comment line format to keep basic information in a plain text table, see the "Gnuastro text table format" section of the book. In short for every column, a comment line like below can be used to give a name, units, comments, or a type to a column. This allows a FITS binary table for example to be written to plain text and converted back to binary without loosing any information (except for very small floating point errors if not enough decimals are printed). # Column N: NAME [UNIT, TYPE, BLANK] COMMENT The new Fits program replaces the old Header program. But besides reading/checking FITS header keywords, it can now also work on FITS extensions/HDUs. For example with no options, it will list all the HDUs in a FITS file along with basic information. It can copy a whole HDU to another file, or delete a HDU from a FITS file. To get the previous behavior of listing all the keywords in a FITS HDU, you can run it with the `-p' option. All programs now write data into the second HDU of a FITS file to allow a clean first HDU. Note that following CFITSIO, HDU counting still starts from zero, so FITS images and tables written by Gnuastro in a new file can always be accessed with the `--hdu=1' option (which is now the default). If any program is run within a Git version controlled directory, a `COMMIT' header keyword will be added to the created FITS files, see the "Output headers" section of the book for a discussion on the usefulness of this new feature. BuildProgram: a new program to easily compile, link and run a C program you have written with Gnuastro's libraries without having to worry about which libraries (Gnuastro dependencies) your program needs. Debugging (`-g'), optimizations (`-O'), warnings (`-W'), include search path (`-I'), link search path (`-L'), and linked libraries (`-l') compiler options are also supported. BuildProgram will greatly facilitate the easy usage of Gnuastro's libraries. ** Removed programs or library features The following program names have been renamed: ImageCrop --> Crop ImageWarp --> Warp ImageStatistics --> Statistics Header --> Fits SubtractSky has been removed. The Statistics program now has tools to estimate the Sky value and it can be subtracted with Arithmetic. ** New features All Gnuastro programs that read and write tables can now do so in plain text table format or in FITS ASCII or FITS Binary tables. Depending on the filename or with the new `--tableformat' common option to all programs. The option management system in all Gnuastro programs has been completely re-written with many new features, some of the most important ones are listed below. For developers, you will notice that there is no more usage of macros and adding new options has become much more easier. -- All programs will now also look for a `gnuastro.conf' configuration file to keep common options for all programs in every directory. -- The `--lastconfig' option can be used on the command-line or in any configuration file to stop parsing any further configuration files. -- The `--config' option can now be used to identify any arbitrary file to be parsed as a configuration file. Any file that is given to this option is parsed immediately. -- The `--printparams' option now also prints the short documentation of each option (same description in `--help') after its value. It is now possible to choose columns in tables based on column names as well as column numbers. It is also possible to search for columns based on searching in their units or comments. When using column numbers, counting now starts from 1 (one), not 0 (as before). See the new "Selecting table columns" section for more on these new features. Where relevant, all programs now accept a `--type' option that you can use to specify the numerical datatype of the output. With the new common option `--minmapsize', you can specify a minimum size of an array (in bytes) to store data in SSD/HDD and not in RAM. This can be instrumental when you are dealing with large datasets, or even smaller ones, but when your RAM is getting full. Making a log file is now optional and users have to explicitly ask for it with the `--log' option. Slower building of Gnuastro: Binary operators (e.g., plus or multiply) are now done in the native type of the input dataset. Doing so for all the different combinations of types, greatly slows down the initial compilation of Gnuastro (after running `make'). So for every type there is now a `--enable-bin-op-*' configure time option. When the dataset's type isn't compiled (only for the binary operators), it will be converted to a compiled type and then converted back in the end. Arithmetic: all operations are done in the native data type of the dataset. Until now, it would convert the data internally to double precision floating point, do the requested operation and write the data back in the proper type. So this new implementation is much more efficient. Arithmetic: two new classes of operators: type conversion operators to all standard types and integer-only operators (all C bit-wise operators and the modulo operator). ConvertType: can also print the input dataset to the command-line (`stdout'). To use this feature set the output filename to `stdout'. Convolve now has the `--minsharpspec' option to specify the minimum spectrum value to use in deconvolution (matching PSFs). Crop: when in WCS mode it can still only work on aligned images. However, very small floating point errors in writing the WCS (for example 10e-13 degrees) are now acceptable. Until now these would cause Crop to complain and abort. Crop: the name of the crop can be pre-determined based on the values in a given in a table column. This allows your object's IDs to be directly used as the crop's file name for example. MakeCatalog now also reports the surface brightness in mag/arcsec^2. Until now, MakeCatalog would only print the dataset's surface brightness in units of magnitudes/pixel. But that is not nicely comparable to other datasets. Hence, using a simple calculation (from the pixel projected size, fully derived in the book), it now also reports the surface brightness in magnitudes/arcsec^2 also. MakeProfiles: Profile codes now start from `1' (until now they started from `0'). MakeProfiles: now accepts the radial function of profiles as human-readable strings instead of a code for each profile (which was very cryptic, although codes are also still acceptable). For example in the profile column you can now write `sersic' instead of the code `1'. NoiseChisel: the new `--cleandilated' option will remove dilated objects that have a low S/N (it is mainly useful on very clean or mock images). For non-clean noise, it will result in a decrease of completeness. With this new option, NoiseChisel will also print detection S/N values when run with the `--checkdetsn' option. Statistics: now reads table columns as well as images and does basic operations on them. It can also only work on a certain range of the data (instead of the whole set). Alternatively, you can define the range on another reference column, but use values of the main column. Statistics: all its single-valued measurements can now be done on a tessellation (tile grid) over the input dataset. Statistics: can now estimate the Sky value on the input dataset using the mode's quantile similar to what NoiseChisel does to find its initial threshold. Statistics: has several new single valued calculations: `--quantile', `--quantfunc' (quantile function), `--mode', `--modequant', `--modesym', and `--modesymvalue'. Warp: align the image with the celestial coordinates using the `--align' option. Warp: standard modular warpings can now be requested without an input matrix, using the following options: `--shear', `--flip', `--project', `--rotate', `--scale', `--translate'. Any number of these transformations (along with the `--align' option) can be called on the command-line and they will be applied in the same order to create one warping matrix. By default the WCS will also be corrected. ** Changes in behavior Mask image options have been removed from all programs. Instead, all programs can work directly on data with blank values. So when some pixels must be masked, the Arithmetic program's `where' operator can be used to select special pixels and set them to blank. In particular bit-wise operations are now available in Arithmetic to use bit-mask images. Managing all these different choices in every program would only confuse the user (with too many options). Arithmetic: the `x' letter is now used to represent the multiplication operator. Previously it was `*' which needed quotation and was thus very inconvenient. Convolve: the old `--frequency' and `--spatial' options have been removed and are replaced by `--domain' which accepts values of `frequency' and `spatial'. Convolve: the old `--viewfreqsteps' was changed to `--checkfreqsteps' to fit with the general style of such check images in all Gnuastro's programs. Crop: `--section' syntax is now inclusive in both bounds. Crop: only checks if the center of a crop is filled when the crop was defined by its center (for example with `--ra' and `--dec'). The verbose outputs of Crop are also not cryptic 0s or 1s. The are human readable text. Crop: doesn't have separate `--imgmode' and `--wcsmode' options any more. There is now a single `--mode' option which accepts values of `img' or `wcs'. MakeProfiles: the old `--inputascanvas' is now called `--clearcanvas'. MakeProfiles: until now, it would abort with an error when the input columns had blank values. But for masking, it might happen that you set a blank magnitude. So this check has now been removed when reading the magnitude column. NoiseChisel: default value of the `--minskyfrac' option (new name for the old `--minbfrac') is now 0.7 as opposed to 0.5. This will allow much better estimation of noise properties (by default). It may be slightly too high for a crowded field, but the users can change it on the command-line (or in a configuration file) for such datasets. NoiseChisel: when it is run with any of the `--check' options, it will abort after all the check images have been created. This is very useful for checking your parameters until each step and not be distracted (or have to wait) for later steps to finish. Statistics: will not make a histogram and cumulative frequency files, or calculate sigma-clipped results by default (with no options). It will just print some basic information. Table: Previously, if a column was requested, the `-i' option would be ignored. But it often happens that the users forget a column name after already typing several of their desired columns. So the opposite behavior is preferred. Because when more than a couple of columns are needed, you will probably forget the column identifiers of the last few and having to retype everything is very frustrating. Something like how `--help' takes precedence over all other options. Table: to select column(s) by regular expression searching, the name now has to be put in `/ /' (similar to AWK). If a value isn't in `/ /', the programs will only select a column with the exact match. Warp: when a 2 by 2 matrix is given, the FITS pixel positions (which define the center of a pixel as an integer) are automatically implemented internally, see "Invoking Warp" in the manual for more. Warp: the old `--nofitscorrect' option has been changed to `--centeroncorner' to be more clear. The new option is now more general than before and also works on warping with a matrix, not just on modular warpings. Warp: the old `--nowcscorrection' option has been given a more clear name of `--keepwcs'. With this option, Warp will not apply the warp the input's WCS structure. Warp: the old `--maxblankfrac' option has been changed to `--coveredfrac'. Until now, Warp would only look for the fraction of input blank/NaN pixel area over the output pixel. But this would be useless on the edges of the image. So the new `--coveredfrac' option takes the acceptable fraction of output pixel area that must be covered by input pixels in order to give that output pixel a value. You can use this to set edge pixels that are not fully covered in the new grid to blank and have a flat warped image. ** Bug fixes Using `%zu' to print `size_t' variables for clean build on 32-bit systems. Crash in Table for some operating systems due to memory is now fixed (bug #49347). Table's man-page is now created and installed (bug #49418). Fixes in the documentation (sr #109170, bug #49419). Check for malloc returning valid pointer (bug #49459). Segfault in mesh interpolation corrected (bug #49588). Corrected bad status usage in calls to wcsp2s and wcss2p (bug #49752). Stricter checking in Crop's polygon point list (bug #48978). Correction in alignment and getting pixel scale (bug #50072). Decomposing PCi_j and CDELTi matrices in output WCS (bug #50073). Using image naxes[n] when checkcenter is larger (bug #50099). Memory leak in MakeCatalog corrected (bug #51118). Fix copy-paste error in MakeCatalog flag arrays (bug #51130). * Noteworthy changes in release 0.2 (library 0.0.0) (2016-10-03) [stable] ** Bug fixes Linker errors on some operating systems have been fixed (bug #48076). Several memory allocation, checks or redundancies have been fixed: bugs #48453, #48516, #48603, #48611, #48571, #48650, #48657, #48692, #48770, #47866, #48899, #49049, #49007. ImageCrop no longer crashes with very long output file names (bugs #46241 and #45380). ** New programs or headers Table: a new utility to read and write FITS binary and ASCII tables. It can also print the column information or select columns using regular expressions (task #13579). Shared libraries and headers are now installed. The libraries can be used in C and C++ programs. This release includes the following headers: `gnuastro.h', `array.h', `box.h', `fits.h', `linkedlist.h', `mesh.h', `polygon.h', `qsort.h', `spatialconvolve.h', `statistics.h', `threads.h', `wcs.h', `txtarray.h' (task #13765). Gnuastro now comes with a script in its top source directory (`tmpfs-config-make') to configure and build it in the tmpfs (on the RAM), for those systems that have it. See the new "Configure and build in RAM" section in the book for more (task #14100). ** New features MakeProfiles also accepts WCS positions (task #13566). Flat profiles in MakeProfiles can be given a profile specific value. The new `--mforflatpix' option MakeProfile will use the value in the magnitude column as a fixed value for each pixel. This can be very useful in defining a mask, or creating segmentation maps or labeled images (task #14115). MakeProfiles can now use input image as canvas. Instead of specifying the WSC and image size parameters manually. With the new `--inputascanvas' option, MakeProfiles will get this information (along with blank pixels) from an already existing image (task #14116). Type of output in MakeProfiles and Arithmetic can be specified with the `--type' option. Magnitude error column in MakeCatalog with the `--magnitudeerr' option. Arithmetic now has new conditional (task #13870) and logical operators (task #14153) along with an operator for actions only when conditions are true: `where'. The new `isblank' operator will also enable you to select blank, or masked, pixels (task #14146). The `--noerodequant' in NoiseChisel enables it to detect small and sharper profiles by disabling erosion on pixels above a certain quantile (task #14139). MakeCatalog can also calculate the upper limit magnitude for each given object in the image by randomly positioning the object's footprint over undetected regions of the image (task #14167). The source tarball is now also distributed with Lzip for a much better compression ratio and more robust archival file format. ** Changes in behavior The two MakeProfiles options `--setconsttonan', `--setconsttomin' have been removed (see `--mforflatpix' above for their alternative). MakeCatalog makes clump catalog only when asked (when the `WCLUMPS' header exists in the objects HDU). This can be very useful in cases like aperture photometry, when the object labels are not generated by NoiseChisel and so a clump image doesn't exist (task #14122). Default cosmological parameters in CosmicCalculator set to Plank 2015 results: A&A (2016), 594, A13 (arXiv 1502.01589). The `--envseed' option (to read random number generator type and seed from the environment) to MakeProfiles and MakeNoise can also be given in the configuration files. * Noteworthy changes in release 0.1 (2016-05-30) [stable] ** Bug fixes MakeCatalog's problem in checking the sizes of all input images is now fixed. NoiseChisel's problem with reading the `--kernel' option is now corrected (bug #46750). lib/mesh.c's problem in correctly calculating the mesh sizes was corrected (bug #47611). `make check' will not look into system utility configuration files. In the previous release, if Gnuastro was already installed, the configuration files already present on the system would also be read. Now only configuration files in the tested package are used (bug #47833). Ghostscript's version is now checked at configure time after its existence. ConvertType uses the `-dPDFFitPage' option to Ghostscript which was introduced in version 9.10, so older versions would pass configure but at `make check' time, the PDF test would fail. Now this test is skipped (bug #47868). Most tests would fail when `make check -jN' was run (to do the checks on N threads). A dependency structure has now been defined to fix this problem and greatly speed up the testing process (bug #47957). ** New utilities Arithmetic: For arithmetic operations on the pixels of input images. With this utility, it is now possible to add multiple images with each other, or easily calculate a median image. It as a large set of other arithmetic operations and some functions which can be done on the input image(s). An unlimited number of input images can be given, the images will only be loaded when necessary and will be freed as soon as they are no longer necessary. CosmicCalculator: For doing cosmological calculations at a given redshift. ** New features All the utilities that would produce a log file now have a `--nolog' option to avoid printing a log file. The tiled image compression convention (.fits.fz, created with `fpack') files can now be used as input in the utilities. ImageCrop can now also crop a polygon from the input image. The polygon vertices can be given in the world or image coordinates. The simple `--polygon' option will keep the insides of the polygon while the `--outpolygon' will keep the outside of the polygon. ImageCrop and ImageWarp can now read the WCS information of a FITS header from a specific region with the `--hstartwcs' and `--hendwcs'. In some older FITS images, when the WCS distortions were not as standardized as now, there were cases which would confuse WCSLIB. NoiseChisel can now save the grown clumps image instead of the original clumps image in the output with the `--grownclumps' option. Convolve can now do deconvolution with the `--makekernel' option. MakeProfiles now has a `--setconsttonan' option which will fill the constant profiles with a NaN (blank) value, not a number, allowing the creations of elliptical masked regions for example. Header can now import a keyword directly from a string with the `--asis' option. MakeCatalog can now output the geometric (average position independent of pixel flux value) positions of the objects too. MakeCatalog can now produce the object's elliptical parameters (for example semi-major axis, semi-minor axis, and position angle). This can also be done both in standard flux weighted and geometric methods too. MakeCatalog now has a `--threshold' function to only use pixels above a given threshold in each object or clump. This is useful to avoid diffuse regions in calculations. MakeCatalog now has a `--noriverbrightness' option. With this option it is possible to calculate the clump flux without subtracting the river pixels on its circumference. The number of CPU threads is no longer a configuration option, it is now determined at run-time for each program. Therefore it is now easily possible to built Gnuastro on one system to use on another (commonly done in the GNU/Linux package managers). Therefore ./configure no longer has a `--with-numthreads' option. Every commit in Gnuastro's history (after implementing this feature) can now be given a unique version number. Since the version number is printed in possible outputs, this feature can help reproducibility, even when the an official/stable release isn't used. The AUTHORS file is now automatically generated from the version controlled history. Also all the authors that have contributed to Gnuastro are included in the second (copyright) page of the PDF book. All the bootstrapped directories are now moved with a new `bootstrapped' directory in the top source directory. This significantly cleans up this directory, allowing users to more easily find the hand-written Gnuastro source files they like. A `bug-gnuastro' Info page was created so users can easily go to that page for information on how to submit bug reports. It is accessible on the command line with the command `info bug-gnuastro'. ** Changes in behavior The separate utilities no longer have a separate version number. With the introduction of unofficial version numbers generated from each commit in Gnuastro's history, the utility version numbers would cause confusion. MakeProfiles will now add a suffix to the individual images and put them in the output directory if specified. NoiseChisel and MakeCatalog now use the median mesh standard deviation to define the over-all depth of the image. Previously they used the maximum value (or the least depth). NoiseChisel no longer outputs a sky subtracted image. This job can now be done with the new Arithmetic utility. NoiseChisel's `--segsnhistnbins' option was renamed to `--clumpsnhistnbins'. ** Improvements NoiseChisel's default quantiles were changed to 0.95 from 0.99. Since the old value was too severe. NoiseChisel's S/N thresholds are now found from the distribution of pseudo-detections and clumps from the full image, not within each large mesh. This was done to increase the accuracy of the S/N threshold. There were commonly not enough points in large mesh sizes and this would add scatter. With ImageCrop's polygon capabilities, it is now easily possible to cut out the region that has uniform noise properties (depth and correlated noise). Therefore the old `--checkdetectionsn' and `checkclumpsn' options are no longer present. When building from the version controlled source, the whole bootstrapping process is done with one script. In the previous version, all the separate operations should have been done by hand (as instructed in the old manual). All the build steps now report what was done and suggest the next step. This feature can be disabled with the `--disable-guide-message' at configure time. gnuastro-0.5/INSTALL0000644000175000017500000003661413217200067011202 00000000000000Installation Instructions ************************* Copyright (C) 1994-1996, 1999-2002, 2004-2016 Free Software Foundation, Inc. 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'--help=short' '--help=recursive' Print a summary of the options unique to this package's 'configure', and exit. The 'short' variant lists options used only in the top level, while the 'recursive' variant lists options also present in any nested packages. '--version' '-V' Print the version of Autoconf used to generate the 'configure' script, and exit. '--cache-file=FILE' Enable the cache: use and save the results of the tests in FILE, traditionally 'config.cache'. FILE defaults to '/dev/null' to disable caching. '--config-cache' '-C' Alias for '--cache-file=config.cache'. '--quiet' '--silent' '-q' Do not print messages saying which checks are being made. To suppress all normal output, redirect it to '/dev/null' (any error messages will still be shown). '--srcdir=DIR' Look for the package's source code in directory DIR. Usually 'configure' can determine that directory automatically. '--prefix=DIR' Use DIR as the installation prefix. *note Installation Names:: for more details, including other options available for fine-tuning the installation locations. '--no-create' '-n' Run the configure checks, but stop before creating any output files. 'configure' also accepts some other, not widely useful, options. Run 'configure --help' for more details. gnuastro-0.5/ChangeLog0000644000175000017500000012014312771240103011711 000000000000002016-05-27 Mohammad Akhlaghi Following the discussions in task #13779, the ChangeLog has not been updated since 2015-11-05 (previous log). Instead, the commit messages are very descriptive. Git's blame tool can be used to check the history of any part of the code very effectively. Gnulib has scripts to generate a ChangeLog from the commit history so building this file automatically is possible and will be implemented (task #14007). Once this ChangeLog is automatically generated, it will be removed from the version controlled source. Until then this file will remain unchanged. There is also a discussion for adopting the ChangeLog format in the commit messages in task #14008. * ChangeLog: no longer updated. 2015-11-05 Mohammad Akhlaghi * doc/gnuastro.texi (Why C): Clarified explanations. 2015-11-04 Mosè Giordano * .gitignore: Add new regexps to the list of ignored files. * doc/gnuastro.texi (Arguments): Mention new accepted extension. * lib/fitsarrayvv.c (nameisfits): Add "fits.fz" to the list of accepted extensions. Fixes task#13767. (nameisfitssuffix): Ditto. 2015-10-18 Mosè Giordano * bin/imgcrop/imgcrop.c (imgcrop): Do not use modefunction to set the function, run the functions manually instead. Fixes bug#45380. 2015-10-16 Mosè Giordano * ./*: Change in many files the name of the package from "gnuastro" to "Gnuastro". Fixes bug#46212. * doc/forwebpage.sh: Use canonical path for bash shell. * doc/plotbin/conversions.sh: Ditto. 2015-10-02 Mohammad Akhlaghi * bin/noisechisel/noisechisel.c (makeoutput): Added a "raw" term in the comments of the noise statistics so emphasize that this is from the raw mesh grid and not the interpolated and smoothed grid. * bin/mkcatalog/mkcatalog.c (makeoutput): As explained below. * doc/gnuastro.texi (Depth and limiting magnitude): Changed the sigma which representes depth from the maximum to the median. The maximum has a strong scatter and even one mesh can completely push to unreasonable values. But the median is not affected by such minor mesh variations, so it is a more robust measure of the dispersion. 2015-10-01 Mohammad Akhlaghi * bin/imgcrop/ui.c (checkifset): Removed the hstartwcs and hendwcs options as mandatory arguments. * lib/fitsarrayvv.c (readfitswcs): Now applies the hstartwcs and hendwcs options. * include/fitsarrayvv.h: readfitswcs now takes the hstartwcs and hendwcs values as arguments. This was done so all programs could take in these options. 2015-09-23 Mohammad Akhlaghi * doc/gnuastro.texi (Depth and limiting magnitude): Updated explanations in for the depth and limiting magnitude to be more realistic. * bin/mkcatalog/mkcatalog.c (makeoutput): Removed the limiting magnitude calculation that was previously defined since it's physical meaning is very unclear (it was mainly put as a test). Also changed the surface brightness limit to a per-pixel basis (independent of the projected area of the pixel) as explained in the manual. 2015-09-17 Mohammad Akhlaghi * bin/mkprof/mkprof.c (mkprof): Only print a log file if the `--nolog' option is not called. * bin/imgcrop/imgcrop.c (imgcrop): Only print a log file if the `--nolog' option is not called. * bin/mkprof/main.h (mkprofparams): Removed the p->dir0file1 parameter from the main structure. * tests/mkprof/mosaic1.sh: Corrected the name of the first output for the new individual name configuration (where the output file name is suffixed to the row number). * bin/mkprof/ui.c (sanitycheck): Now everything based on the situation the basic information for the next steps is set here. * bin/mkprof/mkprof.c (saveindividual): Removed the name checking here. All the necessary information is now set in ui.c. 2015-09-13 Mohammad Akhlaghi * bin/imgwarp/imgwarp.c (imgwarponthread): Now calculates the fraction of area that is blank (NaN) and if that fraction is larger than a user defined value, then the output pixel will be blank. Before the blank fraction was ignored. * bin/imgstat/imgstat.c (reportsimplestats): Now uses the value to the `--mirrordist' option instead of the fixed value of 1.5. (reportsimplestats): Report the `NOT ACCURATE' warning in a separate line to make reading by AWK easier, also removed comma between outputs for the same reason. * bin/*/ui.c (readconfig): Now uses macros for common options. (printvalues): Similarly uses macros for common options. * lib/statistics.c (sigmaclip_converge): Removed commas between the outputs to make reading by AWK easier. (sigmaclip_certainnum): Similar to above. * include/fixedstringmacros.h (GNUASTROBIBTEX): New name from ASTRUTILSBIBTEX. Also the content was updated to the full ADS BibTeX output after the paper was published. * include/configfiles.h (CHECKSETCONFIG): Now checks for the version of the program and also has a more cleaner/readable path for reading/writing to the user configuration directory and reading from the system configuration directory. 2015-08-16 Mohammad Akhlaghi * bin/noisechisel/thresh.c (snthresh): The check on the number of objects in finding the S/N threshold is now done before sorting the S/N table. * bin/convolve/convolve.c (removepaddingcorrectroundoff): When the maximum radius is smaller than the input images, then the final kernel will be shrinked to have no only-zero column or row. 2015-08-05 Mohammad Akhlaghi * bin/convolve/convolve.c (frequencyconvolve): Divide the arrays when the kernel should be made, multiply them when convolution is to be done. (frequencyconvolve): When in deconvolution mode, it will go to another function to make the final product. 2015-07-31 Mohammad Akhlaghi * bin/convolve/convolve.c (makepaddedcomplex): Added a check to make the padded image size an even number in both dimensions by adding one pixel if it is odd. This was done because FFT operations work much faster on even sized arrays. 2015-07-22 Mohammad Akhlaghi * bin/noisechisel/thresh.c (snthresh): Had mistakenly used `p->detquant', for both detection and segmentation! This is now corrected. * bin/mkcatalog/mkcatalog.c (secondpass): Sets the river flux to Sky for when the grown clumps are used, see the explanation bellow. * bin/mkcatalog/columns.c (brightnessmag): Corrected the definition of brightness. It was incorrectly dividing the total brightness by the area when the user asked for brightness. (sncol): Can now work accurately when grown clumps are also included. In a grown clump image, full detections that aren't harmed by deblending are are fully labeled. So there is no river pixels there and the S/N equations had to incorporate this. 2015-07-18 Mohammad Akhlaghi * bin/noisechisel/segmentation.c (nextavailablelabel): Now accounts for the `--grownclumps' option. * bin/noisechisel/args.h (options): Corrected the type of output for `--gthresh'. I had forgot to include any for it! 2015-07-17 Mohammad Akhlaghi * lib/fitsarrayvv.c (pixelareaarcsec2): Previously called pixelsteradians. Changed the units to arcsec^2 because it is more useful. * bin/noisechisel/detection.c (detlabelsn): Now using a new sum of pixel values for flux weighted center of profile. The values are stored as one column in the 2015-07-07 Mohammad Akhlaghi * bin/mkcatalog/mkcatalog.c (firstpass): Use only positive (after subtracting sky) fluxes as weights for the flux weighted center. Also calculate the geometric center (irrespective of flux), so in case there are no positive pixels, the geometric center is output instead (after all, the object should be represented by some position and the NaN values that were used before are not useful). (secondpass): Similar to the above. Also I had simply replaced the getclumpinfo method of NoiseChisel's clumps.c here. But I had forgot that over there, all the neighboring clumps were within one detection. But here, two clumps could be one river pixel appart but belong to separate objects. So the wngb array has to have two values for each clump, not one, see the comments for more. Also I had to check the object IDs from the neighbors, not the river pixel. (setcpscorr): Removed. The minimum and maximum Standard deviations are now stored by NoiseChisel into the header of the standard deviation image. MakeProfiles then gets the value from those header parameters, so there was no need for this function. (makeoutput): The magnitude and S/N information is printed even if the user has not asked for magnitudes and S/Ns. * bin/mkcatalog/columns.c (sncol): Renamed variables to fit the clumpsntable function in bin/noisechisel/clumps.c. Also, the river flux is subtracted here, not before. * lib/fitsarrayvv.c: The numblank variable did not actually store the `number' of blank pixels, it was only a 0 or 1 value to specify if there are any blank pixels or not. It is now changed to `anyblank' to be more clear and not confuse the readers. All the Gnuastro programs that used this variable, were also corrected. 2015-07-06 Mohammad Akhlaghi * bin/noisechisel/noisechisel.c (noisechisel): After dilation, 4 connectivity was used to find the labels of the connected components. However, when we are looking around the river pixels in the segmentation process, we are looking in their 8-connected neighbors. So when two 4-connected labeled regions are separate, they can still be 8-connected and this will mess up the river flux association functions where the flux of a river is given to the clump that is touching it. It took me several frustrating hours to find this very simple bug! * bin/noisechisel/clumps.c (oversegment): NaN (masked) pixels are no longer fed into this function. So the conditions to check for them, especially in setting the top index are removed. (getclumpinfo): Now uses a different number for the sum of flux when trying to find the flux weighted center of the clump. This sum is made of only positive values. Negative values cannot act as weights and will mess up the center calculations. The new number for each column is stored in a third column to the xys array. Also, the xys array is no longer needed outside this function. 2015-07-05 Mohammad Akhlaghi * bin/mkcatalog/columns.c (brightnessfluxmag): Previously fluxmag. Now this function gives the brightness, flux and magnitude depending on its input parameters. * bin/mkcatalog/args.h (options): Corrected all usage of "flux" and "brightness". * doc/gnuastro.texi: Corrected all usage of "flux" and "brightness". * doc/forwebpage.sh (thismonth): Removed type=\"text/javascript\"" from the string since it seemed to be interfering with LibreJS. 2015-07-03 Mohammad Akhlaghi * lib/fitsarrayvv.c (readkeywords): Now reads multiple keywords. 2015-07-02 Mohammad Akhlaghi * bin/mkcatalog/mkcatalog.c (firstpass): Now accounts for blank labeled pixels. (setcpscorr): Now finds both the minimum and maximum of the STD, maximum for finding the 5sigma magnitude. * bin/mkcatalog/main.h (CATUNITMAG): Changed unit for magnitudes. 2015-06-26 Mohammad Akhlaghi * bin/noisechisel/thresh.c (qthreshonmesh): Only sort and find the quantile if there actually is any pixels! (applydetectionthresholdskysub): Now accounts for blank pixels. * bin/noisechisel/segmentation.c (segmentation): Now only works on non-blank pixels. * bin/noisechisel/label.c (BF_concmp): Now accounts for blank pixels in both unsigned char and long arrays. (labareas): Accounts for blank pixels. (removesmallarea_relabel): Accounts for blank pixels. (labindexs): Accounts for blank pixels. * bin/noisechisel/detection.c (detlabelsn): Now also removes detections in the sky area that cover a detection after filling holes. (removefalsedetections): Changed to applydetsn. (detsnthreshonmesh): Changed to detectpsedos. Practically this function just fills the holes in each large mesh and opens the binary result then puts the field back into the main p->dbyt array. It does not calculate anything any more. Such calculations have now become full image wide to find one S/N value over the full image. (detsnthreshongrid): Changed to detsnthresh. This function now does the image-wide calculations that were previously done by detsnthreshonmesh. (dbytolaboverlap): Now accounts for masked unsigned char and long arrays. * bin/noisechisel/clumps.c (clumpsntableonmesh): Previously clumpsnthreshonmesh. Moved all the countings and conditionals to another function to find the S/N threshold from one distribution over the image and not in the large meshs. (findclumpsn): Previously clumpsngrid. Now it collects all the S/N values from all the meshs into one array and uses that to find the S/N threshold using a fixed function for both detection and segmentation (snthresh in thresh.c). * bin/noisechisel/binary.c: The fixed value of 2 is changed BINARYNAN which is defined in binary.h. This makes managing the special values to use more easy, especially now that FITSBYTEBLANK is also being used from fitsarrayvv.h. (fh_makeinv): Replaced the old functions to fill the inverse array with new ones that don't use an index variable but pointers. It is much more cleaner, faster and easier to read now. It also now accounts for blank pixels and completely ignores them. (fillboundedholes): Similar to fh_makeinv. * bin/noisechisel/: The mesh based signal to noise calculations are now gone and one value is calculated for the full image. This allows for much better accuracy. Most of the steps in NoiseChisel were modified to take this into account. Also blank pixels are now included in the binary and labeled images too. * lib/fitsarrayvv.c (arraytofitsimg): Moved the BLANK keyword before EXTNAME. 2015-06-25 Mohammad Akhlaghi * bin/imgcrop/args.h (options): Changed inpolygon to outpolygon. Everywhere that inpolygon appeared, it is now outpolygon. * bin/imgcrop/wcsmode.c (wcscheckprepare): Check for both axises having the same pixel scale now incorporates floating point errors. * bin/imgcrop/crop.c (imgpolygonflpixel): Now gets the vertices and their number instead of the cropparams structure. This was done to make it be more general and use it in both Image mode and WCS mode. (onecrop): Allocation of the crp->ipolygon array was moved to the cropflpixel function. 2015-06-13 Mohammad Akhlaghi * lib/fitsarrayvv.c (fileorextname): New name for the setmaskname function. This was done to be a generic check, for all kinds of input, not just the mask. * bin/ : All the functions to make a copy of an input and print string values were changed. These were mainly in ui.c and args.h for each program. Until now, for each option, I would allocate, check and set the proper values, but now, I wrote a small function in checkset.c (allocatecopyset) which does the job. This makes reading the code significantly more easy and less bugy. 2015-06-12 Mohammad Akhlaghi * bin/subtractsky/args.h (options): Removed the --checkinterpolation option. * bin/subtractsky/subtractsky.c (subtractsky): Similar to below. * bin/noisechisel/thresh.c (findapplyqthreshold): Similar to below. * bin/noisechisel/sky.c (findavestdongrid): Similar to below. * bin/noisechisel/detection.c (findsnthreshongrid): Now using meshvaluefile from mesh.h instead of checking its self. Once the --meshbasedcheck was added, doing all the checks in each function was too long and repetative. So I just made this function to do the job with one call and not distract the readers. 2015-06-11 Mohammad Akhlaghi * bin/noisechisel/args.h (options): `minbfrac' and `minnumfalse' options moved under the `Input' category from the detections category. This move was because these two options are used by both the detection and segmentation steps and thus keeping them under detection would be confusing. Also `checkthresh' was changed to `checkthreshold'. Also, the option `numerosion' was changed to `erode' to be consistent with the opening and dilate options. 2015-06-10 Mohammad Akhlaghi * bin/mknoise/astmknoise.conf: Default background magnitude changed to -10 and zeropoint to 0.0. 2015-06-09 Mohammad Akhlaghi * bin/noisechisel/clumps.c: All functions now use the clumpsthreadparams structure as input instead of a list of arguments. (oversegment): ctp->topinds now keeps a good value when the clump has NaN pixels over it. * lib/mesh.c (imgindextomeshid): Corrected to work correctly when the pixel might be lying on the last mesh that might be larger. 2015-06-08 Mohammad Akhlaghi * bin/noisechisel/thresh.c (applydetectionthresholdskysub): Similar to below, uses p->imgss for sky subtracted image. * bin/noisechisel/sky.c (subtractskyimg): Does not touch the input image, puts the sky subtracted value in p->imgss. * bin/noisechisel/noisechisel.c (noisechisel): Removed the allocation of the mesh structures to ui.c * bin/noisechisel/detection.c (detlabelsn): Uses p->imgss for the sky subtracted image. 2015-06-07 Mohammad Akhlaghi * bin/mkprof/oneprofile.c (randompoints): The random number generator is now allocated (cloned) with the build thread and for every profile the seed is independently set once. Before each pixel would allocate and seed the random number generator individually! * bin/mkprof/astmkprof.conf: Changed default zeropoint magnitude to 0.00. * bin/mknoise/mknoise.c (mknoise): moved the random number generator to ui.c to make things faster and more easier to understand. * bin/mknoise/args.h (argp_option): Removed the `backgroundinmean' option, because I couldn't figure out what use it would have. If it is needed we can add it again later! * bin/imgstat/args.h (argp_option): Changed `binonzero' option to the more general `onebinvalue' option. * bin/convolve/convolve.c (removepaddingcorrectroundoff): Corrected bug: would return *d in both cases! It is corrected now. 2015-06-06 Mohammad Akhlaghi * lib/mesh.c (chbasedidfromgid): Chaged the old setmeshid to chbasedidfromgid along with a new function (gidfromchbasedid). The explanations on top of the first clearly explain everything extensively. The old function (my understanding) was not yet mature enough but now it seems to be very nicely working. All the functions that used this were also changed. * bin/noisechisel/astnoisechisel.conf: Changed default lastmeshfrac to 0.51 from 0.6. 2015-06-04 Mohammad Akhlaghi * bin/subtractsky/subtractsky.c (avestdonthread): No more need for setnan. Since all the meshes are initialized to NaN anyway. * lib/mesh.c: Previously, the garrays would be allocated and freed on every set of operations that were done on the mesh grid. I made some modifications so there is no more need to allocate and free them every time. A new prameter was added (ngarrays) so that on each use of the garrays, the number of garrays that are needed are kept here. All checks to work on the second garray are now done through this parameter. In this fashion, when multiple operations are to done on each mesh, there is no need to repeatedly free and allocate the garrays. Nearly all the functions in mesh.c were corrected to account for this. 2015-06-03 Mohammad Akhlaghi * bin/noisechisel/astnoisechisel.conf: Changed default dthresh to -0.1. * lib/statistics.c (histogram): Corrected the function. Until now, there was a problem when an element was on the last bin: it would go onto the next bin and thus would not be counted. This issue is now corrected. (cumulativefp): Same as above. 2015-06-02 Mohammad Akhlaghi * lib/mesh.c (operateonmesh): mp->indexs is now allocated in makemesh. Because all the programs that will need threads on meshs will need it, so it is best to set mp->indexs once and for all in makemesh. (meshinterponthread): Removed the naninds array, a new option was added to interpolate only on blank pixels when needed. (preparemeshinterparrays): Similar to the above. 2015-06-01 Mohammad Akhlaghi * lib/statistics.c: Removed all isnan checks in the comparison functions for the minimum and maximum values. NaN values will automatically fail all comparisons. * lib/timing.c (reporttiming): Removed the `in' from reporting seconds. * include/timing.h (VERBMSGLENGTH_V): Changed to 45 from 40. 2015-05-27 Mohammad Akhlaghi * bin/convolve/args.h (options): Remove the `noedgecorrection' option. Since it was useless. Also changed the old short option for spatial (`s') to `p'. Because `s' is now needed for the mesh size option. Also changed the old short option for khdu (`H') to `U', to make it similar to all the other programs that do convolution. * include/mesh.h (meshparams): the garrays are now only pointers. The allocated arrays are either cgarrays or fgarrays and based on the user's will, garray will be set equal to one of these two options. All the functions in mesh.c were changed to accomodate this change. 2015-05-25 Mohammad Akhlaghi * lib/mesh.c (operateonmesh): New name for `fillmesh'. Now the function that will be spinned off from each thread can be specified from the outside. 2015-05-24 Mohammad Akhlaghi * bin/imgcrop/crop.c (sectionparser): When only a `*' was given with no positive or negative following number, a segmentation fault would happen. This bug is now fixed. * lib/spatialconvolve.c (sconvonthread): No convolution will be attempted for a NaN pixel. 2015-05-23 Mohammad Akhlaghi * lib/mode.c (modesymmetricity): Corrrected topi to account for the case when 2*mi is larger than size. * bin/subtractsky/args.h: --numnearest and --kernelwidth moved to the `Mesh grid' part of the help output. --checksmoothing and --checkinterpolation also moved to the `Mesh grid' part. * lib/mesh.c (checkgarray): Modified to show both the full, or contiguous over full image, garray and the default one which is contiguous only over each channel. 2015-05-20 Mohammad Akhlaghi * lib/mode.c (modesymmetricity): Corrected topi to the end of the mirror distribution. (modesymmetricity): If no diff point is found, the end of the mirror distribution is used. Before it was the end of the data! (valuefromsym): af set to the quantile of the mirror distribution. 2015-05-18 Mohammad Akhlaghi * bin/convolve/convolve.c (complextoreal): Changed the two states to three to add only conerting the real part of an array. 2015-05-15 Mohammad Akhlaghi * bin/convolve/convolve.c (removepaddingcorrectroundoff): The limit to check for floating point errors is now set by a macro and changed to 1e-10 instead of 1e-17. * lib/statistics.c (sigmaclip_converge): Now, there is a limit on the number of times to try for convergence. * lib/mode.c (makemirrorplots): All the output paramters are now given as arguments so the output can be fully configured from the outside. Also, the method that it sets the plot ranges is now better configurable. * include/mode.h (MODESYMGOOD): Changed to 0.2 from 0.15 based on new simulation tests. 2015-05-11 Mohammad Akhlaghi * lib/statistics.c (setbins): Changed method to find the bin that has the value zero within it. Before it would just choose the first bin with a positive value. But now, it will check the signs of the two interval sides of the bin and when ever the multiplication becomes negative, that bin is chosen. (histogram): Changed so the last bin is a closed bin, not half open like the rest of the histogram bins. This also includes floating point rounding error. (cumulativefp): Same as the histogram function. (sigmaclip_certainnum): Printing is now an option. (sigmaclip_converge): Printing is now an option. * lib/mode.c (makemirrorplots): New name for the old savemodeplots. * include/mode.h: Changed input arguments to modeindexinsorted. Plots can now be made through the separate makemirrorpolots function. 2015-05-05 Mohammad Akhlaghi * bin/subtractsky/ui.c (preparearrays): Moved the function that reads any input as float and incorporates the mask into it. * include/fixedstringmacros.h (MOREHELPINFO): Removed long explanation about help-gnuastro. Instead an info link to the part of the manual that introduces it was included. 2015-05-03 Mohammad Akhlaghi * include/fixedstringmacros.h (MOREHELPINFO): Corrected to include help-gnuastro mailing list. * doc/style.css (a:hover): Changed to bright orange color. (a:active): Changed to dark orange. 2015-04-24 Mohammad Akhlaghi * bin/mkprof/oneprofile.c (makepixbypix): When in circumference mode, if the truncation radius is reached, it is filled with the profile value. This is done so very elongated profiles can at least show a one pixel circumference. * bin/mkprof/main.h (MINCIRCUMWIDTH): Changed to 0.5f. * lib/checkset.c (doublelvalue): Corrected bad value report when options are called. 2015-04-21 Mohammad Akhlaghi * bin/mkprof/ui.c (freeandreport): Avoided double-free by only freeing mergeedimgname when it is not equal to output. * bin/mkprof/oneprofile.c (makepixbypix): Will only do monte carlo integration when the profile is not a constant value. (setprofparams): Changed the function of point to `Fixed'. * bin/mkprof/mkprof.c (write): Changed to replace and read from an image and add profiles on that. * lib/statistics.c: All float and double functions can now work with NaN too. * bin/mkprof/ui.c (setparams): Catalog is always given, no need to check. * doc/gnuastro.texi: Removed all "Future updates ..." subsections in the manual. They are now managed in the Gnuastro project webpage on Savannah. 2015-04-13 Mohammad Akhlaghi * lib/fitsarrayvv.c (updatekeys): When no value is given, it will use fits_update_key_null. (readwcs): Uses fits_free_memory instead of clib's free. 2015-04-06 Mohammad Akhlaghi * bin/mkprof/mkprof.c: Corrected condition when a thread would finish `build' profiles but the last set of its profiles wouldn't pass onto `write'. * bin/mknoise/: Changed background flux unit to magnitudes, not flux. * THANKS: Added institutions which also helped. 2015-04-03 Mohammad Akhlaghi * lib/fitsarrayvv.c: Changed all occurences of `nul' or `NUL' to `blank' or `BLANK'. The FITS standard defines a BLANK keyword for integer types. (copyrightandend): Will now right extra headers. (arraytofitsimg): Can now accept header to write to output. * include/fitsarrayvv.h: Changed all `NUL' macros to `BLANK'. 2015-04-02 Mohammad Akhlaghi * lib/fitsarrayvv.c (changetype): Round floating point input types for integer output types. (arraytofitsimg): Added numblank as a variable, to deal with blank pixels. * bin/imgwarp/imgwarp.c (imgwarppreparations): Coorected the point (1.0f, 1.0f) to be center of the first pixel, not zero. * lib/fitsarrayvv.c (copyrightandend): Removed the Copyright notice of Gnuastro from the output image header. Since it might be confused with a copyright on the data its self. 2015-04-01 Mohammad Akhlaghi * bin/imgwarp/args.h: Temporarily removed the wrap option. Will be added later. 2015-03-24 Mohammad Akhlaghi * bin/imgcrop/ui.c (preparearrays): Aborts if in WCS mode and the wcsprm structure could not be started. * bin/imgcrop/crop.c (firstcropmakearray): Only adds WCS headers if the wcsprm structure is defined. * lib/fitsarrayvv.c (readwcs): If any error occurs, a warning message will be printed and the returned pointer will be NULL. 2015-03-17 Mohammad Akhlaghi * tests/convertt/: If libjpeg is not present, the tests will be skipped. * bin/convertt/: libjpeg is now optional. * configure.ac: Changed libjpeg to an optional requirement. So if it is not available, Gnuastro can still be built. 2015-03-16 Mohammad Akhlaghi * bin/convolve/ui.c (preparearrays): The flip parts was missing a -1. * doc/gnuastro.texi: Changed all `gnuastro' occurrences in the text to `Gnuastro'. 2015-03-14 Mohammad Akhlaghi * bin/convolve/convolve.c: Added frequency domain convolution. 2015-03-12 Mohammad Akhlaghi * bin/mkprof/ui.c (setparams): Added condition for no output given. * bin/mkprof/astmkprof.conf: Removed output. * bin/imgcrop/ui.c (sanitycheck): Moved check of reentrancy in cfitsio to the end so if numthreads is set to 1, there is no problem. * bin/convertt/ui.c (sanitycheck): Added check if output is not set. * bin/convertt/astconvertt.conf: Removed output. * lib/spatialconvolve.c: First version complete. * configure.ac: Removed sqrt and pthread tests (they are done by Gnulib). Added the AX_PTHREAD macro from Autoconf archives. 2015-03-11 Mohammad Akhlaghi * bin/convolve/: Adding new functions and steps. * ./: Copyright transferred to the FSF. Copyright notices in all files changed. 2015-03-10 Mohammad Akhlaghi * tests/imgcrop/*.sh: Set --numthreads=1 for all the tests so if CFITSIO is not installed with reentrancy, there is no failures. * tests/Makefile.am: Made the fitstopdf result conditional on if GPL GhostScript is installed. * include/astrthreads.c: Removed the old function and structure for replacing the pthread_barrier type and functions that was copy and pasted from another webpage and replaced it with my own implementation. * configure.ac: bug report email set. pthread_barrier checked. GPL GhostScript checked. 2015-03-09 Mohammad Akhlaghi * include/astrthreads.h: Added a temporary function so the pthread_barrier type and functions can be run on systems that don't support it. I have contacted the author and it will only remain if he clarifies the license. I have also asked the Gnulib people to try to include it so this issue can be completely fixed. * configure.ac: Added checks for nproc and gs along with warnings. 2015-03-02 Mohammad Akhlaghi * bin/convolve/: Work started on Convolve. * lib/fitsarrayvv.c: Changed array types from intXX_t to short, long and LONGLONG. Unfortuantely this is how CFITSIO works. 2015-02-22 Mohammad Akhlaghi * doc/gnuastro.texi: Added index, changed "Science and its software". 2015-02-20 Mohammad Akhlaghi * doc/gnuastro.texi: Removed list of programs at first, added a programs index. Added an examples chapter along with some one line examples of each program. Moved the Why C and design philosophy subsections to the Developing chapters. * src: All 'error' functions are now called with a string literal and not a string variable. Also all 'system' function calls now check the return value. * lib: Similar to above. * include: similar to above. 2015-02-18 Mohammad Akhlaghi * lib/Makefile.am: Changed all static libraries to libtool static libraries. * doc/gnuastro.texi: Updated. * configure.ac: Added Libtool checks. Corrected cfitsio and wcslib dependencies and removed FFTW as a dependency. 2015-02-17 Mohammad Akhlaghi * bin/convertt/eps.c: Functions for binary image added. * lib/fitsarrayvv.c (nameisfits): Check length. * doc/gnuastro.texi (Internal libraries): Removed details of libraries. * README: Details removed. 2015-02-16 Mohammad Akhlaghi * lib/statistics.c (dminmax): Works with NAN values too. (fminmax): Similar to dminmax. * doc/gnuastro.texi (ConvertType): Updated. 2015-02-13 Mohammad Akhlaghi * bin/convertt/args.h (argp_options): `convert` changed to `change`. Since the program name is also convert this could cause confusions. * doc/gnuastro.texi (Invoking astconvertt): Option explanations. * bin/convertt/jpeg.c (savejpeg): Corrected the pixel ordering. * bin/convertt/convertt.c (doubleto8bit): Find minimum and maximum for all colors to set the scale, not just one color. * lib/fitsarrayvv.c (arraytofitsimg): Will not remove comments. * include/fixedstringmacros.h (SHORTCOPYRIGHT): Corrected year. * lib/fitsarrayvv.c (nameisfits): Dot no longer included. (nameisfitssuffix): Added. (changetype): Corrected input and output pointers. * doc/gnuastro.texi (ConvertType): Added explanations. (Future updates): Chapter removed. 2015-02-11 Mohammad Akhlaghi * bin/convertt/ui.c (preparearrays): Added. * bin/convertt/jpeg.c (preparejpeg): Added. * doc/gnuastro.texi (Files): Added chapter (ConvertType): Added section (FileInfo): Added section 2015-02-08 Mohammad Akhlaghi * bin/convertt: Started working on ConvertType. * lib/checkset.c (intsmallerequalto): Function Added. * include/fixedstringmacros.h (ASTRUTILSBIBTEX): Corrected article name * include/checkset.h: Added intsmallerequalto. 2015-01-25 Mohammad Akhlaghi * ./*: In all files, the name `AstrUtils` was changed to `gnuastro` and the `astr` prefix was changed to `ast`. 2015-01-20 Mohammad Akhlaghi * tests/imgcrop/makerandomcat.py: Removed, because now the points are very specific. * tests/imgcrop/*.sh: Corrected the inputs to the outputs of MakeProfiles tests. * tests/Makefile.am (TESTS): Added tests for MakeProfiles. * Makefile.am (EXTRA_DIST): Moved the distribution files for each folder to the Makefile.am in that folder. 2015-01-19 Mohammad Akhlaghi * bin/mkprof/ui.c: Steps for reading and checking WCS parameters added. * bin/mkprof/oneprofile.c (ispsf): Added for a fixed place to check if a profile is a PSF. (makeoneprofile): Finding mkp->xc and mkp->yc moved here. * bin/mkprof/mkprof.c (preparewcs): Added. (build): Removed finding mkp->xc and mkp->yc. * bin/mkprof/args.h (argp_option): Added WCS related options. * bin/imgcrop/imgcrop.c (imgcrop): Number of barriers, corrected for when the number of jobs was less than the number of threads. * lib/fitsarrayvv.c (addwcstoheader): Changed the WCS structure to the WCS header string as input. (arraytofitsimg): Convert the WCS structure and remove the comments CFITSIO in here. (atofcorrectwcs): Added. * doc/astrutils.texi: Updated. 2015-01-18 Mohammad Akhlaghi * bin/mkprof/mkprof.c (writelog): Added. (write): Completed. * bin/mkprof/args.h (arg_option): Added `--nomerged`. * lib/txtarrayvv.c (doformatting): Added option to use `f` in printf or `g`. 2015-01-16 Mohammad Akhlaghi * bin/mkprof/mkprof.c (builtqueue_addempty): Added. (saveindividual): Added. (build): Is working until the profile is built. * bin/mkprof/ellipse.h: Function taken to `box.h`. * bin/mkprof/ellipse.c: Function taken to `box.c`. * bin/mkprof/args.h (argp_option): added `--numrandom`, changed `mginimg` to `psfinimg`. * bin/imgcrop/main.h (imgcropparams): iwidth is now a 2 element array. * bin/imgcrop/crop.c: Removed `borderfromcenter` and `correctflpixels` to `lib/box.c`. * lib/stats.h: Changed to `statistics.h`, all non-used functions removed. * lib/arraymanip.c: Removed all non-used functions. * include/stats.h: Changed to `statistics.h` and all non-used functions removed. * include/fixedstringmacros.h (ASTRUTILSBIBTEX): Added. * include/commonargs.h (argp_option): Added `--cite` option and added the `main.h` and `cite.h` header for each program to use their names. * include/checkset.h: function name `nameiswritable` is changed to dir0file1 which is much more descriptive. * include/arraymanip.h: Removed all the non-used functions from the past. New functions will be added as they are needed. * doc/astrutils.texi: Updated. 2015-01-13 Mohammad Akhlaghi * bin/mkprof/ui.c (preparearrays): Added. (setparams): numthreads initialized to configured value. * bin/mkprof/mkprof.c (build): Added. (write): Added. (mkprof): Parallel jobs configured. * bin/mkprof/ellipse.c: Added * bin/mkprof/args.h (argp_option): Changed psfprofsinimg to mginimg. * bin/imgcrop/imgcrop.c (imgcrop): Used attrbarrierinit. * lib/astrthreads.c (attrbarrierinit): Added. * doc/astrutils.texi: Updated. 2015-01-12 Mohammad Akhlaghi * bin/imgcrop/imgcrop.c: Using pthread_barrier_wait for synchronizing threads instead of the mutexes and conditional variables before. * lib/txtarrayvv.c: When the value couldn't be read as a number, it would be saved as the lowest possible double value. Now it will be saved as a NaN. * lib/fitsarrayvv.c (nultovalue): Convert blank values in images to a given values. (changetype): Change the type of an image. * lib/checkset.c (nameisawritablefile): Corrected to accurately check if the given name is usable as output. * lib/arraymanip.c (converttofloat): Removed conversion functions. These were mainly for converting a FITS image type to the desired type. Now there is one function in fitsarrayvv.c which will do the conversion. * include/checkset.h (CHECKCOLINCAT): Added to check column number and all values within a column. * doc/astrutils.texi: Updated the text, changing names and explanations. * configure.ac: Changed MockGals, mockgals, name to MakeProfiles, mkprof. * Makefile.am (EXTRA_DIST): Moved the library header files to the Makefile.am in lib/. 2015-01-06 Mohammad Akhlaghi * bin/mockgals/args.h (parse_opt): Removed the check below. * bin/imgcrop/args.h (parse_opt): Removed the check below. * include/commonargs.h (cparse_opt): Added check for not calling `--setdirconf` and `--setusrconf` together. 2015-01-05 Mohammad Akhlaghi * doc/formath.texi: Added. A set of macros to write equations nicely in TeX, HTML (using MathJax). * bin/imgcrop/astrimgcrop.def: renamed to bin/imgcrop/astrimgcrop.conf. * lib/defaults.c: renamed to include/configfiles.c. * lib/checkset.c (stringhasspace): Function added. * include/fixedstringmacros.h (SHORTCOPYRIGHT): 2015 added. (MOREHELPINFO): Corrected info explanation in help output. * include/defaults.h: renamed to include/configfiles.h * include/commonparams.h (commonparams): Similar to the change in commonargs.h. * include/commonargs.h (argp_option): `--dirdefaults` and `--userdefaults` changed to `--setdirconf` and `--setusrconf`. * doc/astrutils.texi: Included formath.texi to display math equations, updates to the text. * doc/Makefile.am (headers): Used a shell '*' instead of calling each program separately. This was enabled with the new file structure. * configure.ac: Changed all default names to configure for a configuration file, not a default file (only name). * Makefile.am: MockGals conditional compilation added. 2014-12-30 Mohammad Akhlaghi * tests/basicchecks.sh: New file (common tests for all tests). * tests/Makefile.am (AM_TESTS_ENVIRONMENT): Corrected test environment. * bin/imgcrop/ui.c (setparams): Moved all similar actions to the CHECKSETDEFAULTS macro in defaults.h * bin/imgcrop/Makefile.am (AM_CPPFLAGS): New (previously in AM_CFLAGS). * lib/defaults.c (addhomedir): Now returns char *. (writelocaldefaultstop): Informs the user of how to make the needed directory with `make -p`. * include/defaults.h (SAVE_LOCAL_DEFAULTS): changed addhomedir. (CHECKSETDEFAULTS): A new macro to read defaults. (END_OF_NOTSET_REPORT): Added some extra information. * doc/astrutils.texi: A lot of updates in the text! Listing them all would be too much! * configure.ac: `--with-numthreads` and `--enable-progname` were created along with all their necessary checks. * Makefile.am: Set conditional subdirectories. Added `basicchecks.sh` to the files to be distributed. 2014-12-28 Mohammad Akhlaghi GNU Astronomical Utilities created with the ImageCrop as the first package. Other packages will be added in the next few days. gnuastro-0.5/COPYING0000644000175000017500000010451312720642724011206 00000000000000 GNU GENERAL PUBLIC LICENSE Version 3, 29 June 2007 Copyright (C) 2007 Free Software Foundation, Inc. Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. Preamble The GNU General Public License is a free, copyleft license for software and other kinds of works. The licenses for most software and other practical works are designed to take away your freedom to share and change the works. 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You may convey verbatim copies of the Program's source code as you receive it, in any medium, provided that you conspicuously and appropriately publish on each copy an appropriate copyright notice; keep intact all notices stating that this License and any non-permissive terms added in accord with section 7 apply to the code; keep intact all notices of the absence of any warranty; and give all recipients a copy of this License along with the Program. You may charge any price or no price for each copy that you convey, and you may offer support or warranty protection for a fee. 5. Conveying Modified Source Versions. You may convey a work based on the Program, or the modifications to produce it from the Program, in the form of source code under the terms of section 4, provided that you also meet all of these conditions: a) The work must carry prominent notices stating that you modified it, and giving a relevant date. b) The work must carry prominent notices stating that it is released under this License and any conditions added under section 7. This requirement modifies the requirement in section 4 to "keep intact all notices". c) You must license the entire work, as a whole, under this License to anyone who comes into possession of a copy. This License will therefore apply, along with any applicable section 7 additional terms, to the whole of the work, and all its parts, regardless of how they are packaged. This License gives no permission to license the work in any other way, but it does not invalidate such permission if you have separately received it. d) If the work has interactive user interfaces, each must display Appropriate Legal Notices; however, if the Program has interactive interfaces that do not display Appropriate Legal Notices, your work need not make them do so. A compilation of a covered work with other separate and independent works, which are not by their nature extensions of the covered work, and which are not combined with it such as to form a larger program, in or on a volume of a storage or distribution medium, is called an "aggregate" if the compilation and its resulting copyright are not used to limit the access or legal rights of the compilation's users beyond what the individual works permit. Inclusion of a covered work in an aggregate does not cause this License to apply to the other parts of the aggregate. 6. Conveying Non-Source Forms. You may convey a covered work in object code form under the terms of sections 4 and 5, provided that you also convey the machine-readable Corresponding Source under the terms of this License, in one of these ways: a) Convey the object code in, or embodied in, a physical product (including a physical distribution medium), accompanied by the Corresponding Source fixed on a durable physical medium customarily used for software interchange. b) Convey the object code in, or embodied in, a physical product (including a physical distribution medium), accompanied by a written offer, valid for at least three years and valid for as long as you offer spare parts or customer support for that product model, to give anyone who possesses the object code either (1) a copy of the Corresponding Source for all the software in the product that is covered by this License, on a durable physical medium customarily used for software interchange, for a price no more than your reasonable cost of physically performing this conveying of source, or (2) access to copy the Corresponding Source from a network server at no charge. c) Convey individual copies of the object code with a copy of the written offer to provide the Corresponding Source. This alternative is allowed only occasionally and noncommercially, and only if you received the object code with such an offer, in accord with subsection 6b. d) Convey the object code by offering access from a designated place (gratis or for a charge), and offer equivalent access to the Corresponding Source in the same way through the same place at no further charge. You need not require recipients to copy the Corresponding Source along with the object code. If the place to copy the object code is a network server, the Corresponding Source may be on a different server (operated by you or a third party) that supports equivalent copying facilities, provided you maintain clear directions next to the object code saying where to find the Corresponding Source. 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If you convey an object code work under this section in, or with, or specifically for use in, a User Product, and the conveying occurs as part of a transaction in which the right of possession and use of the User Product is transferred to the recipient in perpetuity or for a fixed term (regardless of how the transaction is characterized), the Corresponding Source conveyed under this section must be accompanied by the Installation Information. But this requirement does not apply if neither you nor any third party retains the ability to install modified object code on the User Product (for example, the work has been installed in ROM). The requirement to provide Installation Information does not include a requirement to continue to provide support service, warranty, or updates for a work that has been modified or installed by the recipient, or for the User Product in which it has been modified or installed. Access to a network may be denied when the modification itself materially and adversely affects the operation of the network or violates the rules and protocols for communication across the network. Corresponding Source conveyed, and Installation Information provided, in accord with this section must be in a format that is publicly documented (and with an implementation available to the public in source code form), and must require no special password or key for unpacking, reading or copying. 7. Additional Terms. "Additional permissions" are terms that supplement the terms of this License by making exceptions from one or more of its conditions. Additional permissions that are applicable to the entire Program shall be treated as though they were included in this License, to the extent that they are valid under applicable law. If additional permissions apply only to part of the Program, that part may be used separately under those permissions, but the entire Program remains governed by this License without regard to the additional permissions. When you convey a copy of a covered work, you may at your option remove any additional permissions from that copy, or from any part of it. (Additional permissions may be written to require their own removal in certain cases when you modify the work.) You may place additional permissions on material, added by you to a covered work, for which you have or can give appropriate copyright permission. Notwithstanding any other provision of this License, for material you add to a covered work, you may (if authorized by the copyright holders of that material) supplement the terms of this License with terms: a) Disclaiming warranty or limiting liability differently from the terms of sections 15 and 16 of this License; or b) Requiring preservation of specified reasonable legal notices or author attributions in that material or in the Appropriate Legal Notices displayed by works containing it; or c) Prohibiting misrepresentation of the origin of that material, or requiring that modified versions of such material be marked in reasonable ways as different from the original version; or d) Limiting the use for publicity purposes of names of licensors or authors of the material; or e) Declining to grant rights under trademark law for use of some trade names, trademarks, or service marks; or f) Requiring indemnification of licensors and authors of that material by anyone who conveys the material (or modified versions of it) with contractual assumptions of liability to the recipient, for any liability that these contractual assumptions directly impose on those licensors and authors. All other non-permissive additional terms are considered "further restrictions" within the meaning of section 10. If the Program as you received it, or any part of it, contains a notice stating that it is governed by this License along with a term that is a further restriction, you may remove that term. If a license document contains a further restriction but permits relicensing or conveying under this License, you may add to a covered work material governed by the terms of that license document, provided that the further restriction does not survive such relicensing or conveying. If you add terms to a covered work in accord with this section, you must place, in the relevant source files, a statement of the additional terms that apply to those files, or a notice indicating where to find the applicable terms. Additional terms, permissive or non-permissive, may be stated in the form of a separately written license, or stated as exceptions; the above requirements apply either way. 8. Termination. You may not propagate or modify a covered work except as expressly provided under this License. Any attempt otherwise to propagate or modify it is void, and will automatically terminate your rights under this License (including any patent licenses granted under the third paragraph of section 11). However, if you cease all violation of this License, then your license from a particular copyright holder is reinstated (a) provisionally, unless and until the copyright holder explicitly and finally terminates your license, and (b) permanently, if the copyright holder fails to notify you of the violation by some reasonable means prior to 60 days after the cessation. Moreover, your license from a particular copyright holder is reinstated permanently if the copyright holder notifies you of the violation by some reasonable means, this is the first time you have received notice of violation of this License (for any work) from that copyright holder, and you cure the violation prior to 30 days after your receipt of the notice. Termination of your rights under this section does not terminate the licenses of parties who have received copies or rights from you under this License. If your rights have been terminated and not permanently reinstated, you do not qualify to receive new licenses for the same material under section 10. 9. Acceptance Not Required for Having Copies. You are not required to accept this License in order to receive or run a copy of the Program. Ancillary propagation of a covered work occurring solely as a consequence of using peer-to-peer transmission to receive a copy likewise does not require acceptance. However, nothing other than this License grants you permission to propagate or modify any covered work. These actions infringe copyright if you do not accept this License. Therefore, by modifying or propagating a covered work, you indicate your acceptance of this License to do so. 10. Automatic Licensing of Downstream Recipients. Each time you convey a covered work, the recipient automatically receives a license from the original licensors, to run, modify and propagate that work, subject to this License. You are not responsible for enforcing compliance by third parties with this License. An "entity transaction" is a transaction transferring control of an organization, or substantially all assets of one, or subdividing an organization, or merging organizations. If propagation of a covered work results from an entity transaction, each party to that transaction who receives a copy of the work also receives whatever licenses to the work the party's predecessor in interest had or could give under the previous paragraph, plus a right to possession of the Corresponding Source of the work from the predecessor in interest, if the predecessor has it or can get it with reasonable efforts. You may not impose any further restrictions on the exercise of the rights granted or affirmed under this License. For example, you may not impose a license fee, royalty, or other charge for exercise of rights granted under this License, and you may not initiate litigation (including a cross-claim or counterclaim in a lawsuit) alleging that any patent claim is infringed by making, using, selling, offering for sale, or importing the Program or any portion of it. 11. Patents. A "contributor" is a copyright holder who authorizes use under this License of the Program or a work on which the Program is based. The work thus licensed is called the contributor's "contributor version". A contributor's "essential patent claims" are all patent claims owned or controlled by the contributor, whether already acquired or hereafter acquired, that would be infringed by some manner, permitted by this License, of making, using, or selling its contributor version, but do not include claims that would be infringed only as a consequence of further modification of the contributor version. For purposes of this definition, "control" includes the right to grant patent sublicenses in a manner consistent with the requirements of this License. Each contributor grants you a non-exclusive, worldwide, royalty-free patent license under the contributor's essential patent claims, to make, use, sell, offer for sale, import and otherwise run, modify and propagate the contents of its contributor version. In the following three paragraphs, a "patent license" is any express agreement or commitment, however denominated, not to enforce a patent (such as an express permission to practice a patent or covenant not to sue for patent infringement). To "grant" such a patent license to a party means to make such an agreement or commitment not to enforce a patent against the party. If you convey a covered work, knowingly relying on a patent license, and the Corresponding Source of the work is not available for anyone to copy, free of charge and under the terms of this License, through a publicly available network server or other readily accessible means, then you must either (1) cause the Corresponding Source to be so available, or (2) arrange to deprive yourself of the benefit of the patent license for this particular work, or (3) arrange, in a manner consistent with the requirements of this License, to extend the patent license to downstream recipients. "Knowingly relying" means you have actual knowledge that, but for the patent license, your conveying the covered work in a country, or your recipient's use of the covered work in a country, would infringe one or more identifiable patents in that country that you have reason to believe are valid. If, pursuant to or in connection with a single transaction or arrangement, you convey, or propagate by procuring conveyance of, a covered work, and grant a patent license to some of the parties receiving the covered work authorizing them to use, propagate, modify or convey a specific copy of the covered work, then the patent license you grant is automatically extended to all recipients of the covered work and works based on it. A patent license is "discriminatory" if it does not include within the scope of its coverage, prohibits the exercise of, or is conditioned on the non-exercise of one or more of the rights that are specifically granted under this License. You may not convey a covered work if you are a party to an arrangement with a third party that is in the business of distributing software, under which you make payment to the third party based on the extent of your activity of conveying the work, and under which the third party grants, to any of the parties who would receive the covered work from you, a discriminatory patent license (a) in connection with copies of the covered work conveyed by you (or copies made from those copies), or (b) primarily for and in connection with specific products or compilations that contain the covered work, unless you entered into that arrangement, or that patent license was granted, prior to 28 March 2007. Nothing in this License shall be construed as excluding or limiting any implied license or other defenses to infringement that may otherwise be available to you under applicable patent law. 12. No Surrender of Others' Freedom. If conditions are imposed on you (whether by court order, agreement or otherwise) that contradict the conditions of this License, they do not excuse you from the conditions of this License. If you cannot convey a covered work so as to satisfy simultaneously your obligations under this License and any other pertinent obligations, then as a consequence you may not convey it at all. For example, if you agree to terms that obligate you to collect a royalty for further conveying from those to whom you convey the Program, the only way you could satisfy both those terms and this License would be to refrain entirely from conveying the Program. 13. Use with the GNU Affero General Public License. Notwithstanding any other provision of this License, you have permission to link or combine any covered work with a work licensed under version 3 of the GNU Affero General Public License into a single combined work, and to convey the resulting work. The terms of this License will continue to apply to the part which is the covered work, but the special requirements of the GNU Affero General Public License, section 13, concerning interaction through a network will apply to the combination as such. 14. Revised Versions of this License. The Free Software Foundation may publish revised and/or new versions of the GNU General Public License from time to time. Such new versions will be similar in spirit to the present version, but may differ in detail to address new problems or concerns. Each version is given a distinguishing version number. If the Program specifies that a certain numbered version of the GNU General Public License "or any later version" applies to it, you have the option of following the terms and conditions either of that numbered version or of any later version published by the Free Software Foundation. If the Program does not specify a version number of the GNU General Public License, you may choose any version ever published by the Free Software Foundation. If the Program specifies that a proxy can decide which future versions of the GNU General Public License can be used, that proxy's public statement of acceptance of a version permanently authorizes you to choose that version for the Program. Later license versions may give you additional or different permissions. However, no additional obligations are imposed on any author or copyright holder as a result of your choosing to follow a later version. 15. Disclaimer of Warranty. THERE IS NO WARRANTY FOR THE PROGRAM, TO THE EXTENT PERMITTED BY APPLICABLE LAW. EXCEPT WHEN OTHERWISE STATED IN WRITING THE COPYRIGHT HOLDERS AND/OR OTHER PARTIES PROVIDE THE PROGRAM "AS IS" WITHOUT WARRANTY OF ANY KIND, EITHER EXPRESSED OR IMPLIED, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE. THE ENTIRE RISK AS TO THE QUALITY AND PERFORMANCE OF THE PROGRAM IS WITH YOU. SHOULD THE PROGRAM PROVE DEFECTIVE, YOU ASSUME THE COST OF ALL NECESSARY SERVICING, REPAIR OR CORRECTION. 16. Limitation of Liability. IN NO EVENT UNLESS REQUIRED BY APPLICABLE LAW OR AGREED TO IN WRITING WILL ANY COPYRIGHT HOLDER, OR ANY OTHER PARTY WHO MODIFIES AND/OR CONVEYS THE PROGRAM AS PERMITTED ABOVE, BE LIABLE TO YOU FOR DAMAGES, INCLUDING ANY GENERAL, SPECIAL, INCIDENTAL OR CONSEQUENTIAL DAMAGES ARISING OUT OF THE USE OR INABILITY TO USE THE PROGRAM (INCLUDING BUT NOT LIMITED TO LOSS OF DATA OR DATA BEING RENDERED INACCURATE OR LOSSES SUSTAINED BY YOU OR THIRD PARTIES OR A FAILURE OF THE PROGRAM TO OPERATE WITH ANY OTHER PROGRAMS), EVEN IF SUCH HOLDER OR OTHER PARTY HAS BEEN ADVISED OF THE POSSIBILITY OF SUCH DAMAGES. 17. Interpretation of Sections 15 and 16. If the disclaimer of warranty and limitation of liability provided above cannot be given local legal effect according to their terms, reviewing courts shall apply local law that most closely approximates an absolute waiver of all civil liability in connection with the Program, unless a warranty or assumption of liability accompanies a copy of the Program in return for a fee. END OF TERMS AND CONDITIONS How to Apply These Terms to Your New Programs If you develop a new program, and you want it to be of the greatest possible use to the public, the best way to achieve this is to make it free software which everyone can redistribute and change under these terms. To do so, attach the following notices to the program. It is safest to attach them to the start of each source file to most effectively state the exclusion of warranty; and each file should have at least the "copyright" line and a pointer to where the full notice is found. Copyright (C) This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . Also add information on how to contact you by electronic and paper mail. If the program does terminal interaction, make it output a short notice like this when it starts in an interactive mode: Copyright (C) This program comes with ABSOLUTELY NO WARRANTY; for details type `show w'. This is free software, and you are welcome to redistribute it under certain conditions; type `show c' for details. The hypothetical commands `show w' and `show c' should show the appropriate parts of the General Public License. Of course, your program's commands might be different; for a GUI interface, you would use an "about box". You should also get your employer (if you work as a programmer) or school, if any, to sign a "copyright disclaimer" for the program, if necessary. For more information on this, and how to apply and follow the GNU GPL, see . The GNU General Public License does not permit incorporating your program into proprietary programs. If your program is a subroutine library, you may consider it more useful to permit linking proprietary applications with the library. If this is what you want to do, use the GNU Lesser General Public License instead of this License. But first, please read . gnuastro-0.5/AUTHORS0000644000175000017500000000062113217220023011200 00000000000000GNU Astronomy Utilities (Gnuastro) authors ========================================== Generated for Gnuastro 0.5. Ordered by number of commits in the Git project history. 883 Mohammad Akhlaghi 29 Mosè Giordano 18 Vladimir Markelov 7 Boud Roukema 1 Lucas MacQuarrie gnuastro-0.5/config.h.in0000644000175000017500000024172013217217704012176 00000000000000/* config.h.in. Generated from configure.ac by autoheader. */ /* CPU and C ABI indicator */ #ifndef __i386__ #undef __i386__ #endif #ifndef __x86_64_x32__ #undef __x86_64_x32__ #endif #ifndef __x86_64__ #undef __x86_64__ #endif #ifndef __alpha__ #undef __alpha__ #endif #ifndef __arm__ #undef __arm__ #endif #ifndef __armhf__ #undef __armhf__ #endif #ifndef __arm64_ilp32__ #undef __arm64_ilp32__ #endif #ifndef __arm64__ #undef __arm64__ #endif #ifndef __hppa__ #undef __hppa__ #endif #ifndef __hppa64__ #undef __hppa64__ #endif #ifndef __ia64_ilp32__ #undef __ia64_ilp32__ #endif #ifndef __ia64__ #undef __ia64__ #endif #ifndef __m68k__ #undef __m68k__ #endif #ifndef __mips__ #undef __mips__ #endif #ifndef __mipsn32__ #undef __mipsn32__ #endif #ifndef __mips64__ #undef __mips64__ #endif #ifndef __powerpc__ #undef __powerpc__ #endif #ifndef __powerpc64__ #undef __powerpc64__ #endif #ifndef __powerpc64_elfv2__ #undef __powerpc64_elfv2__ #endif #ifndef __s390__ #undef __s390__ #endif #ifndef __s390x__ #undef __s390x__ #endif #ifndef __sh__ #undef __sh__ #endif #ifndef __sparc__ #undef __sparc__ #endif #ifndef __sparc64__ #undef __sparc64__ #endif /* Define if building universal (internal helper macro) */ #undef AC_APPLE_UNIVERSAL_BUILD /* Define to the number of bits in type 'ptrdiff_t'. */ #undef BITSIZEOF_PTRDIFF_T /* Define to the number of bits in type 'sig_atomic_t'. */ #undef BITSIZEOF_SIG_ATOMIC_T /* Define to the number of bits in type 'size_t'. */ #undef BITSIZEOF_SIZE_T /* Define to the number of bits in type 'wchar_t'. */ #undef BITSIZEOF_WCHAR_T /* Define to the number of bits in type 'wint_t'. */ #undef BITSIZEOF_WINT_T /* Configuration file post fix. */ #undef CONF_POSTFIX /* Configuration file name format. */ #undef CONF_SHOWFMT /* Define to one of `_getb67', `GETB67', `getb67' for Cray-2 and Cray-YMP systems. This function is required for `alloca.c' support on those systems. */ #undef CRAY_STACKSEG_END /* Define to 1 if using `alloca.c'. */ #undef C_ALLOCA /* Define to 1 if the C locale may have encoding errors. */ #undef C_LOCALE_MAYBE_EILSEQ /* Define as the bit index in the word where to find bit 0 of the exponent of 'double'. */ #undef DBL_EXPBIT0_BIT /* Define as the word index where to find the exponent of 'double'. */ #undef DBL_EXPBIT0_WORD /* Define as the bit index in the word where to find the sign of 'double'. */ #undef DBL_SIGNBIT_BIT /* Define as the word index where to find the sign of 'double'. */ #undef DBL_SIGNBIT_WORD /* Define to 1 if // is a file system root distinct from /. */ #undef DOUBLE_SLASH_IS_DISTINCT_ROOT /* Define this to 1 if F_DUPFD behavior does not match POSIX */ #undef FCNTL_DUPFD_BUGGY /* Define to nothing if C supports flexible array members, and to 1 if it does not. That way, with a declaration like 'struct s { int n; double d[FLEXIBLE_ARRAY_MEMBER]; };', the struct hack can be used with pre-C99 compilers. When computing the size of such an object, don't use 'sizeof (struct s)' as it overestimates the size. Use 'offsetof (struct s, d)' instead. Don't use 'offsetof (struct s, d[0])', as this doesn't work with MSVC and with C++ compilers. */ #undef FLEXIBLE_ARRAY_MEMBER /* Define as the bit index in the word where to find bit 0 of the exponent of 'float'. */ #undef FLT_EXPBIT0_BIT /* Define as the word index where to find the exponent of 'float'. */ #undef FLT_EXPBIT0_WORD /* Define as the bit index in the word where to find the sign of 'float'. */ #undef FLT_SIGNBIT_BIT /* Define as the word index where to find the sign of 'float'. */ #undef FLT_SIGNBIT_WORD /* Define to 1 if nl_langinfo (YESEXPR) returns a non-empty string. */ #undef FUNC_NL_LANGINFO_YESEXPR_WORKS /* The executable to call GNU Libtool */ #undef GAL_CONFIG_GNULIBTOOL_EXEC /* libgit2 is installed on the system */ #undef GAL_CONFIG_HAVE_LIBGIT2 /* System has pthread_barrier */ #undef GAL_CONFIG_HAVE_PTHREAD_BARRIER /* WCSLIB comes with wcslib_version */ #undef GAL_CONFIG_HAVE_WCSLIB_VERSION /* On 32bit will be 4, on 64 bit, will be 8 */ #undef GAL_CONFIG_SIZEOF_LONG /* On 32bit will be 4, on 64 bit, will be 8 */ #undef GAL_CONFIG_SIZEOF_SIZE_T /* Define if gettimeofday clobbers the localtime buffer. */ #undef GETTIMEOFDAY_CLOBBERS_LOCALTIME /* Define this to 'void' or 'struct timezone' to match the system's declaration of the second argument to gettimeofday. */ #undef GETTIMEOFDAY_TIMEZONE /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module fscanf shall be considered present. */ #undef GNULIB_FSCANF /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module lock shall be considered present. */ #undef GNULIB_LOCK /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module malloc-gnu shall be considered present. */ #undef GNULIB_MALLOC_GNU /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module msvc-nothrow shall be considered present. */ #undef GNULIB_MSVC_NOTHROW /* Define to 1 if printf and friends should be labeled with attribute "__gnu_printf__" instead of "__printf__" */ #undef GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU /* Define to 1 to add extern declaration of program_invocation_name to argp.h */ #undef GNULIB_PROGRAM_INVOCATION_NAME /* Define to 1 to add extern declaration of program_invocation_short_name to argp.h */ #undef GNULIB_PROGRAM_INVOCATION_SHORT_NAME /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module scanf shall be considered present. */ #undef GNULIB_SCANF /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module strerror shall be considered present. */ #undef GNULIB_STRERROR /* Define to a C preprocessor expression that evaluates to 1 or 0, depending whether the gnulib module strerror_r-posix shall be considered present. */ #undef GNULIB_STRERROR_R_POSIX /* Define to 1 when the gnulib module accept should be tested. */ #undef GNULIB_TEST_ACCEPT /* Define to 1 when the gnulib module bind should be tested. */ #undef GNULIB_TEST_BIND /* Define to 1 when the gnulib module btowc should be tested. */ #undef GNULIB_TEST_BTOWC /* Define to 1 when the gnulib module cloexec should be tested. */ #undef GNULIB_TEST_CLOEXEC /* Define to 1 when the gnulib module close should be tested. */ #undef GNULIB_TEST_CLOSE /* Define to 1 when the gnulib module connect should be tested. */ #undef GNULIB_TEST_CONNECT /* Define to 1 when the gnulib module dup2 should be tested. */ #undef GNULIB_TEST_DUP2 /* Define to 1 when the gnulib module environ should be tested. */ #undef GNULIB_TEST_ENVIRON /* Define to 1 when the gnulib module fcntl should be tested. */ #undef GNULIB_TEST_FCNTL /* Define to 1 when the gnulib module fdopen should be tested. */ #undef GNULIB_TEST_FDOPEN /* Define to 1 when the gnulib module fstat should be tested. */ #undef GNULIB_TEST_FSTAT /* Define to 1 when the gnulib module ftruncate should be tested. */ #undef GNULIB_TEST_FTRUNCATE /* Define to 1 when the gnulib module getcwd should be tested. */ #undef GNULIB_TEST_GETCWD /* Define to 1 when the gnulib module getdelim should be tested. */ #undef GNULIB_TEST_GETDELIM /* Define to 1 when the gnulib module getdtablesize should be tested. */ #undef GNULIB_TEST_GETDTABLESIZE /* Define to 1 when the gnulib module getline should be tested. */ #undef GNULIB_TEST_GETLINE /* Define to 1 when the gnulib module getpagesize should be tested. */ #undef GNULIB_TEST_GETPAGESIZE /* Define to 1 when the gnulib module gettimeofday should be tested. */ #undef GNULIB_TEST_GETTIMEOFDAY /* Define to 1 when the gnulib module ioctl should be tested. */ #undef GNULIB_TEST_IOCTL /* Define to 1 when the gnulib module iswblank should be tested. */ #undef GNULIB_TEST_ISWBLANK /* Define to 1 when the gnulib module listen should be tested. */ #undef GNULIB_TEST_LISTEN /* Define to 1 when the gnulib module localeconv should be tested. */ #undef GNULIB_TEST_LOCALECONV /* Define to 1 when the gnulib module lstat should be tested. */ #undef GNULIB_TEST_LSTAT /* Define to 1 when the gnulib module malloc-posix should be tested. */ #undef GNULIB_TEST_MALLOC_POSIX /* Define to 1 when the gnulib module mbrtowc should be tested. */ #undef GNULIB_TEST_MBRTOWC /* Define to 1 when the gnulib module mbschr should be tested. */ #undef GNULIB_TEST_MBSCHR /* Define to 1 when the gnulib module mbsinit should be tested. */ #undef GNULIB_TEST_MBSINIT /* Define to 1 when the gnulib module mbspbrk should be tested. */ #undef GNULIB_TEST_MBSPBRK /* Define to 1 when the gnulib module mbsspn should be tested. */ #undef GNULIB_TEST_MBSSPN /* Define to 1 when the gnulib module mbstok_r should be tested. */ #undef GNULIB_TEST_MBSTOK_R /* Define to 1 when the gnulib module mbtowc should be tested. */ #undef GNULIB_TEST_MBTOWC /* Define to 1 when the gnulib module memchr should be tested. */ #undef GNULIB_TEST_MEMCHR /* Define to 1 when the gnulib module mempcpy should be tested. */ #undef GNULIB_TEST_MEMPCPY /* Define to 1 when the gnulib module nanosleep should be tested. */ #undef GNULIB_TEST_NANOSLEEP /* Define to 1 when the gnulib module nl_langinfo should be tested. */ #undef GNULIB_TEST_NL_LANGINFO /* Define to 1 when the gnulib module open should be tested. */ #undef GNULIB_TEST_OPEN /* Define to 1 when the gnulib module perror should be tested. */ #undef GNULIB_TEST_PERROR /* Define to 1 when the gnulib module pipe should be tested. */ #undef GNULIB_TEST_PIPE /* Define to 1 when the gnulib module pthread_sigmask should be tested. */ #undef GNULIB_TEST_PTHREAD_SIGMASK /* Define to 1 when the gnulib module putenv should be tested. */ #undef GNULIB_TEST_PUTENV /* Define to 1 when the gnulib module raise should be tested. */ #undef GNULIB_TEST_RAISE /* Define to 1 when the gnulib module rawmemchr should be tested. */ #undef GNULIB_TEST_RAWMEMCHR /* Define to 1 when the gnulib module select should be tested. */ #undef GNULIB_TEST_SELECT /* Define to 1 when the gnulib module setenv should be tested. */ #undef GNULIB_TEST_SETENV /* Define to 1 when the gnulib module setlocale should be tested. */ #undef GNULIB_TEST_SETLOCALE /* Define to 1 when the gnulib module setsockopt should be tested. */ #undef GNULIB_TEST_SETSOCKOPT /* Define to 1 when the gnulib module sigaction should be tested. */ #undef GNULIB_TEST_SIGACTION /* Define to 1 when the gnulib module signbit should be tested. */ #undef GNULIB_TEST_SIGNBIT /* Define to 1 when the gnulib module sigprocmask should be tested. */ #undef GNULIB_TEST_SIGPROCMASK /* Define to 1 when the gnulib module sleep should be tested. */ #undef GNULIB_TEST_SLEEP /* Define to 1 when the gnulib module socket should be tested. */ #undef GNULIB_TEST_SOCKET /* Define to 1 when the gnulib module stat should be tested. */ #undef GNULIB_TEST_STAT /* Define to 1 when the gnulib module strchrnul should be tested. */ #undef GNULIB_TEST_STRCHRNUL /* Define to 1 when the gnulib module strerror should be tested. */ #undef GNULIB_TEST_STRERROR /* Define to 1 when the gnulib module strerror_r should be tested. */ #undef GNULIB_TEST_STRERROR_R /* Define to 1 when the gnulib module strndup should be tested. */ #undef GNULIB_TEST_STRNDUP /* Define to 1 when the gnulib module strnlen should be tested. */ #undef GNULIB_TEST_STRNLEN /* Define to 1 when the gnulib module strtod should be tested. */ #undef GNULIB_TEST_STRTOD /* Define to 1 when the gnulib module strtok_r should be tested. */ #undef GNULIB_TEST_STRTOK_R /* Define to 1 when the gnulib module symlink should be tested. */ #undef GNULIB_TEST_SYMLINK /* Define to 1 when the gnulib module unsetenv should be tested. */ #undef GNULIB_TEST_UNSETENV /* Define to 1 when the gnulib module usleep should be tested. */ #undef GNULIB_TEST_USLEEP /* Define to 1 when the gnulib module vsnprintf should be tested. */ #undef GNULIB_TEST_VSNPRINTF /* Define to 1 when the gnulib module wcrtomb should be tested. */ #undef GNULIB_TEST_WCRTOMB /* Define to 1 when the gnulib module wctob should be tested. */ #undef GNULIB_TEST_WCTOB /* Define to 1 when the gnulib module wctomb should be tested. */ #undef GNULIB_TEST_WCTOMB /* Define to 1 when the gnulib module wcwidth should be tested. */ #undef GNULIB_TEST_WCWIDTH /* Define to 1 if you have 'alloca' after including , a header that may be supplied by this distribution. */ #undef HAVE_ALLOCA /* Define to 1 if you have and it should be used (not on Ultrix). */ #undef HAVE_ALLOCA_H /* Define to 1 if you have the header file. */ #undef HAVE_ARPA_INET_H /* Define to 1 if you have the header file. */ #undef HAVE_BP_SYM_H /* Define to 1 if you have the `btowc' function. */ #undef HAVE_BTOWC /* Define to 1 if nanosleep mishandles large arguments. */ #undef HAVE_BUG_BIG_NANOSLEEP /* Define to 1 if you have the `catgets' function. */ #undef HAVE_CATGETS /* Define to 1 if you have the Mac OS X function CFLocaleCopyCurrent in the CoreFoundation framework. */ #undef HAVE_CFLOCALECOPYCURRENT /* Define to 1 if you have the Mac OS X function CFPreferencesCopyAppValue in the CoreFoundation framework. */ #undef HAVE_CFPREFERENCESCOPYAPPVALUE /* Define to 1 if you have the `chsize' function. */ #undef HAVE_CHSIZE /* Define if the copysignf function is declared in and available in libc. */ #undef HAVE_COPYSIGNF_IN_LIBC /* Define if the copysignl function is declared in and available in libc. */ #undef HAVE_COPYSIGNL_IN_LIBC /* Define if the copysign function is declared in and available in libc. */ #undef HAVE_COPYSIGN_IN_LIBC /* Define to 1 if you have the header file. */ #undef HAVE_CRTDEFS_H /* Define to 1 if you have the declaration of `alarm', and to 0 if you don't. */ #undef HAVE_DECL_ALARM /* Define to 1 if you have the declaration of `clearerr_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_CLEARERR_UNLOCKED /* Define to 1 if you have the declaration of `copysign', and to 0 if you don't. */ #undef HAVE_DECL_COPYSIGN /* Define to 1 if you have the declaration of `copysignf', and to 0 if you don't. */ #undef HAVE_DECL_COPYSIGNF /* Define to 1 if you have the declaration of `copysignl', and to 0 if you don't. */ #undef HAVE_DECL_COPYSIGNL /* Define to 1 if you have the declaration of `feof_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FEOF_UNLOCKED /* Define to 1 if you have the declaration of `ferror_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FERROR_UNLOCKED /* Define to 1 if you have the declaration of `fflush_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FFLUSH_UNLOCKED /* Define to 1 if you have the declaration of `fgets_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FGETS_UNLOCKED /* Define to 1 if you have the declaration of `fputc_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FPUTC_UNLOCKED /* Define to 1 if you have the declaration of `fputs_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FPUTS_UNLOCKED /* Define to 1 if you have the declaration of `fread_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FREAD_UNLOCKED /* Define to 1 if you have the declaration of `fwrite_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_FWRITE_UNLOCKED /* Define to 1 if you have the declaration of `getchar_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_GETCHAR_UNLOCKED /* Define to 1 if you have the declaration of `getc_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_GETC_UNLOCKED /* Define to 1 if you have the declaration of `getdelim', and to 0 if you don't. */ #undef HAVE_DECL_GETDELIM /* Define to 1 if you have the declaration of `getdtablesize', and to 0 if you don't. */ #undef HAVE_DECL_GETDTABLESIZE /* Define to 1 if you have the declaration of `getline', and to 0 if you don't. */ #undef HAVE_DECL_GETLINE /* Define to 1 if you have the declaration of `inet_pton', and to 0 if you don't. */ #undef HAVE_DECL_INET_PTON /* Define to 1 if you have the declaration of `isblank', and to 0 if you don't. */ #undef HAVE_DECL_ISBLANK /* Define to 1 if you have the declaration of `iswblank', and to 0 if you don't. */ #undef HAVE_DECL_ISWBLANK /* Define to 1 if you have the declaration of `mbrtowc', and to 0 if you don't. */ #undef HAVE_DECL_MBRTOWC /* Define to 1 if you have the declaration of `mbsinit', and to 0 if you don't. */ #undef HAVE_DECL_MBSINIT /* Define to 1 if you have the declaration of `program_invocation_name', and to 0 if you don't. */ #undef HAVE_DECL_PROGRAM_INVOCATION_NAME /* Define to 1 if you have the declaration of `program_invocation_short_name', and to 0 if you don't. */ #undef HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME /* Define to 1 if you have the declaration of `putchar_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_PUTCHAR_UNLOCKED /* Define to 1 if you have the declaration of `putc_unlocked', and to 0 if you don't. */ #undef HAVE_DECL_PUTC_UNLOCKED /* Define to 1 if you have the declaration of `setenv', and to 0 if you don't. */ #undef HAVE_DECL_SETENV /* Define to 1 if you have the declaration of `sleep', and to 0 if you don't. */ #undef HAVE_DECL_SLEEP /* Define to 1 if you have the declaration of `strerror_r', and to 0 if you don't. */ #undef HAVE_DECL_STRERROR_R /* Define to 1 if you have the declaration of `strncasecmp', and to 0 if you don't. */ #undef HAVE_DECL_STRNCASECMP /* Define to 1 if you have the declaration of `strndup', and to 0 if you don't. */ #undef HAVE_DECL_STRNDUP /* Define to 1 if you have the declaration of `strnlen', and to 0 if you don't. */ #undef HAVE_DECL_STRNLEN /* Define to 1 if you have the declaration of `strtok_r', and to 0 if you don't. */ #undef HAVE_DECL_STRTOK_R /* Define to 1 if you have the declaration of `towlower', and to 0 if you don't. */ #undef HAVE_DECL_TOWLOWER /* Define to 1 if you have the declaration of `unsetenv', and to 0 if you don't. */ #undef HAVE_DECL_UNSETENV /* Define to 1 if you have the declaration of `vsnprintf', and to 0 if you don't. */ #undef HAVE_DECL_VSNPRINTF /* Define to 1 if you have the declaration of `wcrtomb', and to 0 if you don't. */ #undef HAVE_DECL_WCRTOMB /* Define to 1 if you have the declaration of `wctob', and to 0 if you don't. */ #undef HAVE_DECL_WCTOB /* Define to 1 if you have the declaration of `wcwidth', and to 0 if you don't. */ #undef HAVE_DECL_WCWIDTH /* Define to 1 if you have the declaration of `_putenv', and to 0 if you don't. */ #undef HAVE_DECL__PUTENV /* Define to 1 if you have the declaration of `_snprintf', and to 0 if you don't. */ #undef HAVE_DECL__SNPRINTF /* Define to 1 if you have the declaration of `__argv', and to 0 if you don't. */ #undef HAVE_DECL___ARGV /* Define to 1 if you have the header file. */ #undef HAVE_DLFCN_H /* Define to 1 if you have the 'dup2' function. */ #undef HAVE_DUP2 /* Define if you have the declaration of environ. */ #undef HAVE_ENVIRON_DECL /* Define to 1 if you have the `fcntl' function. */ #undef HAVE_FCNTL /* Define to 1 if you have the header file. */ #undef HAVE_FEATURES_H /* Define to 1 if you have the `flockfile' function. */ #undef HAVE_FLOCKFILE /* Define to 1 if you have the `ftruncate' function. */ #undef HAVE_FTRUNCATE /* Define to 1 if you have the `funlockfile' function. */ #undef HAVE_FUNLOCKFILE /* Define to 1 if you have the `getdelim' function. */ #undef HAVE_GETDELIM /* Define to 1 if you have the `getdtablesize' function. */ #undef HAVE_GETDTABLESIZE /* Define to 1 if you have the `getexecname' function. */ #undef HAVE_GETEXECNAME /* Define to 1 if you have the `getlocalename_l' function. */ #undef HAVE_GETLOCALENAME_L /* Define to 1 if you have the header file. */ #undef HAVE_GETOPT_H /* Define to 1 if you have the `getopt_long_only' function. */ #undef HAVE_GETOPT_LONG_ONLY /* Define to 1 if you have the `getpagesize' function. */ #undef HAVE_GETPAGESIZE /* Define to 1 if you have the `getprogname' function. */ #undef HAVE_GETPROGNAME /* Define to 1 if you have the `gettimeofday' function. */ #undef HAVE_GETTIMEOFDAY /* Define to 1 if you have the `inet_pton' function. */ #undef HAVE_INET_PTON /* Define if you have the 'intmax_t' type in or . */ #undef HAVE_INTMAX_T /* Define to 1 if you have the header file. */ #undef HAVE_INTTYPES_H /* Define if exists, doesn't clash with , and declares uintmax_t. */ #undef HAVE_INTTYPES_H_WITH_UINTMAX /* Define to 1 if you have the `ioctl' function. */ #undef HAVE_IOCTL /* Define to 1 if defines AF_INET. */ #undef HAVE_IPV4 /* Define to 1 if defines AF_INET6. */ #undef HAVE_IPV6 /* Define to 1 if you have the `isblank' function. */ #undef HAVE_ISBLANK /* Define if the isnan(double) function is available in libc. */ #undef HAVE_ISNAND_IN_LIBC /* Define if the isnan(float) function is available in libc. */ #undef HAVE_ISNANF_IN_LIBC /* Define if the isnan(long double) function is available in libc. */ #undef HAVE_ISNANL_IN_LIBC /* Define to 1 if you have the `iswblank' function. */ #undef HAVE_ISWBLANK /* Define to 1 if you have the `iswcntrl' function. */ #undef HAVE_ISWCNTRL /* Define to 1 if you have the `iswctype' function. */ #undef HAVE_ISWCTYPE /* Define if you have and nl_langinfo(CODESET). */ #undef HAVE_LANGINFO_CODESET /* Define to 1 if you have the header file. */ #undef HAVE_LANGINFO_H /* Define if your file defines LC_MESSAGES. */ #undef HAVE_LC_MESSAGES /* Define if the ldexp function is available in libc. */ #undef HAVE_LDEXP_IN_LIBC /* Define to 1 if you have the header file. */ #undef HAVE_LIBINTL_H /* Has libjpeg */ #undef HAVE_LIBJPEG /* Define to 1 if you have the header file. */ #undef HAVE_LIMITS_H /* Define to 1 if you have the header file. */ #undef HAVE_LINEWRAP_H /* Define to 1 if the system has the type 'long long int'. */ #undef HAVE_LONG_LONG_INT /* Define to 1 if you have the `lstat' function. */ #undef HAVE_LSTAT /* Define to 1 if your system has a GNU libc compatible `malloc' function, and to 0 otherwise. */ #undef HAVE_MALLOC /* Define to 1 if your system has a GNU libc compatible 'malloc' function, and to 0 otherwise. */ #undef HAVE_MALLOC_GNU /* Define to 1 if you have the header file. */ #undef HAVE_MALLOC_H /* Define if the 'malloc' function is POSIX compliant. */ #undef HAVE_MALLOC_POSIX /* Define to 1 if mmap()'s MAP_ANONYMOUS flag is available after including config.h and . */ #undef HAVE_MAP_ANONYMOUS /* Define to 1 if you have the header file. */ #undef HAVE_MATH_H /* Define to 1 if you have the `mbrtowc' function. */ #undef HAVE_MBRTOWC /* Define to 1 if you have the `mbsinit' function. */ #undef HAVE_MBSINIT /* Define to 1 if declares mbstate_t. */ #undef HAVE_MBSTATE_T /* Define to 1 if you have the header file. */ #undef HAVE_MEMORY_H /* Define to 1 if you have the `mempcpy' function. */ #undef HAVE_MEMPCPY /* Define to 1 if defines the MIN and MAX macros. */ #undef HAVE_MINMAX_IN_LIMITS_H /* Define to 1 if defines the MIN and MAX macros. */ #undef HAVE_MINMAX_IN_SYS_PARAM_H /* Define to 1 if you have the `mprotect' function. */ #undef HAVE_MPROTECT /* Define to 1 on MSVC platforms that have the "invalid parameter handler" concept. */ #undef HAVE_MSVC_INVALID_PARAMETER_HANDLER /* Define to 1 if you have the header file. */ #undef HAVE_NETDB_H /* Define to 1 if you have the header file. */ #undef HAVE_NETINET_IN_H /* Define to 1 if you have the `newlocale' function. */ #undef HAVE_NEWLOCALE /* Define to 1 if you have the `nl_langinfo' function. */ #undef HAVE_NL_LANGINFO /* Define to 1 if you have the header file. */ #undef HAVE_OS_H /* Define to 1 if you have the `pipe' function. */ #undef HAVE_PIPE /* Define if program_invocation_name is defined */ #undef HAVE_PROGRAM_INVOCATION_NAME /* Define if program_invocation_short_name is defined */ #undef HAVE_PROGRAM_INVOCATION_SHORT_NAME /* Define to 1 if you have the `pstat_getdynamic' function. */ #undef HAVE_PSTAT_GETDYNAMIC /* Define if you have POSIX threads libraries and header files. */ #undef HAVE_PTHREAD /* Define to 1 if you have the `pthread_atfork' function. */ #undef HAVE_PTHREAD_ATFORK /* Define if the defines PTHREAD_MUTEX_RECURSIVE. */ #undef HAVE_PTHREAD_MUTEX_RECURSIVE /* Have PTHREAD_PRIO_INHERIT. */ #undef HAVE_PTHREAD_PRIO_INHERIT /* Define if the POSIX multithreading library has read/write locks. */ #undef HAVE_PTHREAD_RWLOCK /* Define if the 'pthread_rwlock_rdlock' function prefers a writer to a reader. */ #undef HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER /* Define to 1 if the pthread_sigmask function can be used (despite bugs). */ #undef HAVE_PTHREAD_SIGMASK /* Define to 1 if you have the `raise' function. */ #undef HAVE_RAISE /* Define to 1 if you have the `rawmemchr' function. */ #undef HAVE_RAWMEMCHR /* Define to 1 if accept is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ACCEPT /* Define to 1 if accept4 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ACCEPT4 /* Define to 1 if acosf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ACOSF /* Define to 1 if acosl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ACOSL /* Define to 1 if asinf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ASINF /* Define to 1 if asinl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ASINL /* Define to 1 if atanf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ATANF /* Define to 1 if atanl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ATANL /* Define to 1 if atoll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ATOLL /* Define to 1 if bind is declared even after undefining macros. */ #undef HAVE_RAW_DECL_BIND /* Define to 1 if btowc is declared even after undefining macros. */ #undef HAVE_RAW_DECL_BTOWC /* Define to 1 if canonicalize_file_name is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CANONICALIZE_FILE_NAME /* Define to 1 if cbrt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CBRT /* Define to 1 if cbrtf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CBRTF /* Define to 1 if cbrtl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CBRTL /* Define to 1 if ceilf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CEILF /* Define to 1 if ceill is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CEILL /* Define to 1 if chdir is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CHDIR /* Define to 1 if chown is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CHOWN /* Define to 1 if connect is declared even after undefining macros. */ #undef HAVE_RAW_DECL_CONNECT /* Define to 1 if copysign is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COPYSIGN /* Define to 1 if copysignf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COPYSIGNF /* Define to 1 if copysignl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COPYSIGNL /* Define to 1 if cosf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COSF /* Define to 1 if coshf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COSHF /* Define to 1 if cosl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_COSL /* Define to 1 if dprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DPRINTF /* Define to 1 if dup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUP /* Define to 1 if dup2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUP2 /* Define to 1 if dup3 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUP3 /* Define to 1 if duplocale is declared even after undefining macros. */ #undef HAVE_RAW_DECL_DUPLOCALE /* Define to 1 if endusershell is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ENDUSERSHELL /* Define to 1 if environ is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ENVIRON /* Define to 1 if euidaccess is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EUIDACCESS /* Define to 1 if exp2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXP2 /* Define to 1 if exp2f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXP2F /* Define to 1 if exp2l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXP2L /* Define to 1 if expf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPF /* Define to 1 if expl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPL /* Define to 1 if expm1 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPM1 /* Define to 1 if expm1f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPM1F /* Define to 1 if expm1l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_EXPM1L /* Define to 1 if fabsf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FABSF /* Define to 1 if fabsl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FABSL /* Define to 1 if faccessat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FACCESSAT /* Define to 1 if fchdir is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCHDIR /* Define to 1 if fchmodat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCHMODAT /* Define to 1 if fchownat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCHOWNAT /* Define to 1 if fcntl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FCNTL /* Define to 1 if fdatasync is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FDATASYNC /* Define to 1 if ffs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FFS /* Define to 1 if ffsl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FFSL /* Define to 1 if ffsll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FFSLL /* Define to 1 if floorf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FLOORF /* Define to 1 if floorl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FLOORL /* Define to 1 if fma is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMA /* Define to 1 if fmaf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMAF /* Define to 1 if fmal is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMAL /* Define to 1 if fmod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMOD /* Define to 1 if fmodf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMODF /* Define to 1 if fmodl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FMODL /* Define to 1 if fpurge is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FPURGE /* Define to 1 if frexpf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FREXPF /* Define to 1 if frexpl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FREXPL /* Define to 1 if fseeko is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSEEKO /* Define to 1 if fstat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSTAT /* Define to 1 if fstatat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSTATAT /* Define to 1 if fsync is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FSYNC /* Define to 1 if ftello is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FTELLO /* Define to 1 if ftruncate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FTRUNCATE /* Define to 1 if futimens is declared even after undefining macros. */ #undef HAVE_RAW_DECL_FUTIMENS /* Define to 1 if getcwd is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETCWD /* Define to 1 if getdelim is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETDELIM /* Define to 1 if getdomainname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETDOMAINNAME /* Define to 1 if getdtablesize is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETDTABLESIZE /* Define to 1 if getgroups is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETGROUPS /* Define to 1 if gethostname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETHOSTNAME /* Define to 1 if getline is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLINE /* Define to 1 if getloadavg is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLOADAVG /* Define to 1 if getlogin is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLOGIN /* Define to 1 if getlogin_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETLOGIN_R /* Define to 1 if getpagesize is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETPAGESIZE /* Define to 1 if getpeername is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETPEERNAME /* Define to 1 if gets is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETS /* Define to 1 if getsockname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETSOCKNAME /* Define to 1 if getsockopt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETSOCKOPT /* Define to 1 if getsubopt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETSUBOPT /* Define to 1 if gettimeofday is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETTIMEOFDAY /* Define to 1 if getusershell is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GETUSERSHELL /* Define to 1 if grantpt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GRANTPT /* Define to 1 if group_member is declared even after undefining macros. */ #undef HAVE_RAW_DECL_GROUP_MEMBER /* Define to 1 if hypotf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_HYPOTF /* Define to 1 if hypotl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_HYPOTL /* Define to 1 if ilogb is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ILOGB /* Define to 1 if ilogbf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ILOGBF /* Define to 1 if ilogbl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ILOGBL /* Define to 1 if imaxabs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_IMAXABS /* Define to 1 if imaxdiv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_IMAXDIV /* Define to 1 if inet_ntop is declared even after undefining macros. */ #undef HAVE_RAW_DECL_INET_NTOP /* Define to 1 if inet_pton is declared even after undefining macros. */ #undef HAVE_RAW_DECL_INET_PTON /* Define to 1 if initstate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_INITSTATE /* Define to 1 if initstate_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_INITSTATE_R /* Define to 1 if ioctl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_IOCTL /* Define to 1 if isatty is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ISATTY /* Define to 1 if isblank is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ISBLANK /* Define to 1 if iswctype is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ISWCTYPE /* Define to 1 if lchmod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LCHMOD /* Define to 1 if lchown is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LCHOWN /* Define to 1 if ldexpf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LDEXPF /* Define to 1 if ldexpl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LDEXPL /* Define to 1 if link is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LINK /* Define to 1 if linkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LINKAT /* Define to 1 if listen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LISTEN /* Define to 1 if log is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG /* Define to 1 if log10 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG10 /* Define to 1 if log10f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG10F /* Define to 1 if log10l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG10L /* Define to 1 if log1p is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG1P /* Define to 1 if log1pf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG1PF /* Define to 1 if log1pl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG1PL /* Define to 1 if log2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG2 /* Define to 1 if log2f is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG2F /* Define to 1 if log2l is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOG2L /* Define to 1 if logb is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGB /* Define to 1 if logbf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGBF /* Define to 1 if logbl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGBL /* Define to 1 if logf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGF /* Define to 1 if logl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LOGL /* Define to 1 if lseek is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LSEEK /* Define to 1 if lstat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_LSTAT /* Define to 1 if mbrlen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBRLEN /* Define to 1 if mbrtowc is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBRTOWC /* Define to 1 if mbsinit is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBSINIT /* Define to 1 if mbsnrtowcs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBSNRTOWCS /* Define to 1 if mbsrtowcs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MBSRTOWCS /* Define to 1 if memmem is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MEMMEM /* Define to 1 if mempcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MEMPCPY /* Define to 1 if memrchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MEMRCHR /* Define to 1 if mkdirat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKDIRAT /* Define to 1 if mkdtemp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKDTEMP /* Define to 1 if mkfifo is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKFIFO /* Define to 1 if mkfifoat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKFIFOAT /* Define to 1 if mknod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKNOD /* Define to 1 if mknodat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKNODAT /* Define to 1 if mkostemp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKOSTEMP /* Define to 1 if mkostemps is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKOSTEMPS /* Define to 1 if mkstemp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKSTEMP /* Define to 1 if mkstemps is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MKSTEMPS /* Define to 1 if modf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MODF /* Define to 1 if modff is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MODFF /* Define to 1 if modfl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_MODFL /* Define to 1 if nl_langinfo is declared even after undefining macros. */ #undef HAVE_RAW_DECL_NL_LANGINFO /* Define to 1 if openat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_OPENAT /* Define to 1 if pclose is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PCLOSE /* Define to 1 if pipe is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PIPE /* Define to 1 if pipe2 is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PIPE2 /* Define to 1 if popen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_POPEN /* Define to 1 if posix_openpt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_POSIX_OPENPT /* Define to 1 if powf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_POWF /* Define to 1 if pread is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PREAD /* Define to 1 if pselect is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PSELECT /* Define to 1 if pthread_sigmask is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PTHREAD_SIGMASK /* Define to 1 if ptsname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PTSNAME /* Define to 1 if ptsname_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PTSNAME_R /* Define to 1 if pwrite is declared even after undefining macros. */ #undef HAVE_RAW_DECL_PWRITE /* Define to 1 if qsort_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_QSORT_R /* Define to 1 if random is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RANDOM /* Define to 1 if random_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RANDOM_R /* Define to 1 if rawmemchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RAWMEMCHR /* Define to 1 if readlink is declared even after undefining macros. */ #undef HAVE_RAW_DECL_READLINK /* Define to 1 if readlinkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_READLINKAT /* Define to 1 if reallocarray is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REALLOCARRAY /* Define to 1 if realpath is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REALPATH /* Define to 1 if recv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RECV /* Define to 1 if recvfrom is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RECVFROM /* Define to 1 if remainder is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REMAINDER /* Define to 1 if remainderf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REMAINDERF /* Define to 1 if remainderl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_REMAINDERL /* Define to 1 if renameat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RENAMEAT /* Define to 1 if rint is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RINT /* Define to 1 if rintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RINTF /* Define to 1 if rintl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RINTL /* Define to 1 if rmdir is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RMDIR /* Define to 1 if round is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ROUND /* Define to 1 if roundf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ROUNDF /* Define to 1 if roundl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_ROUNDL /* Define to 1 if rpmatch is declared even after undefining macros. */ #undef HAVE_RAW_DECL_RPMATCH /* Define to 1 if secure_getenv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SECURE_GETENV /* Define to 1 if select is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SELECT /* Define to 1 if send is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SEND /* Define to 1 if sendto is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SENDTO /* Define to 1 if setenv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETENV /* Define to 1 if sethostname is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETHOSTNAME /* Define to 1 if setlocale is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETLOCALE /* Define to 1 if setsockopt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETSOCKOPT /* Define to 1 if setstate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETSTATE /* Define to 1 if setstate_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETSTATE_R /* Define to 1 if setusershell is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SETUSERSHELL /* Define to 1 if shutdown is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SHUTDOWN /* Define to 1 if sigaction is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGACTION /* Define to 1 if sigaddset is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGADDSET /* Define to 1 if sigdelset is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGDELSET /* Define to 1 if sigemptyset is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGEMPTYSET /* Define to 1 if sigfillset is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGFILLSET /* Define to 1 if sigismember is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGISMEMBER /* Define to 1 if sigpending is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGPENDING /* Define to 1 if sigprocmask is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SIGPROCMASK /* Define to 1 if sinf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SINF /* Define to 1 if sinhf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SINHF /* Define to 1 if sinl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SINL /* Define to 1 if sleep is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SLEEP /* Define to 1 if snprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SNPRINTF /* Define to 1 if socket is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SOCKET /* Define to 1 if sqrtf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SQRTF /* Define to 1 if sqrtl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SQRTL /* Define to 1 if srandom is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SRANDOM /* Define to 1 if srandom_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SRANDOM_R /* Define to 1 if stat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STAT /* Define to 1 if stpcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STPCPY /* Define to 1 if stpncpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STPNCPY /* Define to 1 if strcasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRCASECMP /* Define to 1 if strcasestr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRCASESTR /* Define to 1 if strchrnul is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRCHRNUL /* Define to 1 if strdup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRDUP /* Define to 1 if strerror_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRERROR_R /* Define to 1 if strncasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNCASECMP /* Define to 1 if strncat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNCAT /* Define to 1 if strndup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNDUP /* Define to 1 if strnlen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRNLEN /* Define to 1 if strpbrk is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRPBRK /* Define to 1 if strsep is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRSEP /* Define to 1 if strsignal is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRSIGNAL /* Define to 1 if strtod is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOD /* Define to 1 if strtoimax is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOIMAX /* Define to 1 if strtok_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOK_R /* Define to 1 if strtoll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOLL /* Define to 1 if strtoull is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOULL /* Define to 1 if strtoumax is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRTOUMAX /* Define to 1 if strverscmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_STRVERSCMP /* Define to 1 if symlink is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SYMLINK /* Define to 1 if symlinkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_SYMLINKAT /* Define to 1 if tanf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TANF /* Define to 1 if tanhf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TANHF /* Define to 1 if tanl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TANL /* Define to 1 if tmpfile is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TMPFILE /* Define to 1 if towctrans is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TOWCTRANS /* Define to 1 if trunc is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNC /* Define to 1 if truncate is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNCATE /* Define to 1 if truncf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNCF /* Define to 1 if truncl is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TRUNCL /* Define to 1 if ttyname_r is declared even after undefining macros. */ #undef HAVE_RAW_DECL_TTYNAME_R /* Define to 1 if unlink is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNLINK /* Define to 1 if unlinkat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNLINKAT /* Define to 1 if unlockpt is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNLOCKPT /* Define to 1 if unsetenv is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UNSETENV /* Define to 1 if usleep is declared even after undefining macros. */ #undef HAVE_RAW_DECL_USLEEP /* Define to 1 if utimensat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_UTIMENSAT /* Define to 1 if vdprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_VDPRINTF /* Define to 1 if vsnprintf is declared even after undefining macros. */ #undef HAVE_RAW_DECL_VSNPRINTF /* Define to 1 if wcpcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCPCPY /* Define to 1 if wcpncpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCPNCPY /* Define to 1 if wcrtomb is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCRTOMB /* Define to 1 if wcscasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCASECMP /* Define to 1 if wcscat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCAT /* Define to 1 if wcschr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCHR /* Define to 1 if wcscmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCMP /* Define to 1 if wcscoll is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCOLL /* Define to 1 if wcscpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCPY /* Define to 1 if wcscspn is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSCSPN /* Define to 1 if wcsdup is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSDUP /* Define to 1 if wcsftime is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSFTIME /* Define to 1 if wcslen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSLEN /* Define to 1 if wcsncasecmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCASECMP /* Define to 1 if wcsncat is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCAT /* Define to 1 if wcsncmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCMP /* Define to 1 if wcsncpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNCPY /* Define to 1 if wcsnlen is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNLEN /* Define to 1 if wcsnrtombs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSNRTOMBS /* Define to 1 if wcspbrk is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSPBRK /* Define to 1 if wcsrchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSRCHR /* Define to 1 if wcsrtombs is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSRTOMBS /* Define to 1 if wcsspn is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSSPN /* Define to 1 if wcsstr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSSTR /* Define to 1 if wcstok is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSTOK /* Define to 1 if wcswidth is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSWIDTH /* Define to 1 if wcsxfrm is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCSXFRM /* Define to 1 if wctob is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCTOB /* Define to 1 if wctrans is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCTRANS /* Define to 1 if wctype is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCTYPE /* Define to 1 if wcwidth is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WCWIDTH /* Define to 1 if wmemchr is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMCHR /* Define to 1 if wmemcmp is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMCMP /* Define to 1 if wmemcpy is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMCPY /* Define to 1 if wmemmove is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMMOVE /* Define to 1 if wmemset is declared even after undefining macros. */ #undef HAVE_RAW_DECL_WMEMSET /* Define to 1 if _Exit is declared even after undefining macros. */ #undef HAVE_RAW_DECL__EXIT /* Define to 1 if 'long double' and 'double' have the same representation. */ #undef HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Define to 1 if the system has the type `sa_family_t'. */ #undef HAVE_SA_FAMILY_T /* Define to 1 if you have the `sched_getaffinity' function. */ #undef HAVE_SCHED_GETAFFINITY /* Define to 1 if sched_getaffinity has a glibc compatible declaration. */ #undef HAVE_SCHED_GETAFFINITY_LIKE_GLIBC /* Define to 1 if you have the `sched_getaffinity_np' function. */ #undef HAVE_SCHED_GETAFFINITY_NP /* Define to 1 if you have the header file. */ #undef HAVE_SEARCH_H /* Define to 1 if you have the header file. */ #undef HAVE_SEMAPHORE_H /* Define to 1 if you have the `setdtablesize' function. */ #undef HAVE_SETDTABLESIZE /* Define to 1 if you have the `setenv' function. */ #undef HAVE_SETENV /* Define to 1 if you have the `setlocale' function. */ #undef HAVE_SETLOCALE /* Define to 1 if you have the `shutdown' function. */ #undef HAVE_SHUTDOWN /* Define to 1 if you have the `sigaction' function. */ #undef HAVE_SIGACTION /* Define to 1 if you have the `sigaltstack' function. */ #undef HAVE_SIGALTSTACK /* Define to 1 if the system has the type `siginfo_t'. */ #undef HAVE_SIGINFO_T /* Define to 1 if you have the `siginterrupt' function. */ #undef HAVE_SIGINTERRUPT /* Define to 1 if 'sig_atomic_t' is a signed integer type. */ #undef HAVE_SIGNED_SIG_ATOMIC_T /* Define to 1 if 'wchar_t' is a signed integer type. */ #undef HAVE_SIGNED_WCHAR_T /* Define to 1 if 'wint_t' is a signed integer type. */ #undef HAVE_SIGNED_WINT_T /* Define to 1 if the system has the type `sigset_t'. */ #undef HAVE_SIGSET_T /* Define to 1 if you have the `sleep' function. */ #undef HAVE_SLEEP /* Define to 1 if you have the `snprintf' function. */ #undef HAVE_SNPRINTF /* Define if the return value of the snprintf function is the number of of bytes (excluding the terminating NUL) that would have been produced if the buffer had been large enough. */ #undef HAVE_SNPRINTF_RETVAL_C99 /* Define to 1 if you have the header file. */ #undef HAVE_STDINT_H /* Define if exists, doesn't clash with , and declares uintmax_t. */ #undef HAVE_STDINT_H_WITH_UINTMAX /* Define to 1 if you have the header file. */ #undef HAVE_STDLIB_H /* Define to 1 if you have the `strcasecmp' function. */ #undef HAVE_STRCASECMP /* Define to 1 if you have the `strchrnul' function. */ #undef HAVE_STRCHRNUL /* Define to 1 if you have the `strerror_r' function. */ #undef HAVE_STRERROR_R /* Define to 1 if you have the header file. */ #undef HAVE_STRINGS_H /* Define to 1 if you have the header file. */ #undef HAVE_STRING_H /* Define to 1 if you have the `strncasecmp' function. */ #undef HAVE_STRNCASECMP /* Define to 1 if you have the `strndup' function. */ #undef HAVE_STRNDUP /* Define to 1 if you have the `strnlen' function. */ #undef HAVE_STRNLEN /* Define to 1 if you have the `strtok_r' function. */ #undef HAVE_STRTOK_R /* Define to 1 if `decimal_point' is a member of `struct lconv'. */ #undef HAVE_STRUCT_LCONV_DECIMAL_POINT /* Define to 1 if `sa_sigaction' is a member of `struct sigaction'. */ #undef HAVE_STRUCT_SIGACTION_SA_SIGACTION /* Define to 1 if the system has the type `struct sockaddr_storage'. */ #undef HAVE_STRUCT_SOCKADDR_STORAGE /* Define to 1 if `ss_family' is a member of `struct sockaddr_storage'. */ #undef HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY /* Define to 1 if `st_atimensec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_ATIMENSEC /* Define to 1 if `st_atimespec.tv_nsec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_ATIMESPEC_TV_NSEC /* Define to 1 if `st_atim.st__tim.tv_nsec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_ATIM_ST__TIM_TV_NSEC /* Define to 1 if `st_atim.tv_nsec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_ATIM_TV_NSEC /* Define to 1 if `st_birthtimensec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_BIRTHTIMENSEC /* Define to 1 if `st_birthtimespec.tv_nsec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_BIRTHTIMESPEC_TV_NSEC /* Define to 1 if `st_birthtim.tv_nsec' is a member of `struct stat'. */ #undef HAVE_STRUCT_STAT_ST_BIRTHTIM_TV_NSEC /* Define to 1 if you have the `symlink' function. */ #undef HAVE_SYMLINK /* Define to 1 if you have the `sysctl' function. */ #undef HAVE_SYSCTL /* Define to 1 if you have the header file. */ #undef HAVE_SYSEXITS_H /* Define to 1 if you have the `sysmp' function. */ #undef HAVE_SYSMP /* Define to 1 if you have the header file. */ #undef HAVE_SYS_BITYPES_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_CDEFS_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_INTTYPES_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_IOCTL_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_MMAN_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_PARAM_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_PSTAT_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SELECT_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SOCKET_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_STAT_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SYSCTL_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_SYSMP_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_TIME_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_TYPES_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_UIO_H /* Define to 1 if you have the header file. */ #undef HAVE_SYS_WAIT_H /* Define to 1 if you have the `towlower' function. */ #undef HAVE_TOWLOWER /* Define to 1 if you have the `tsearch' function. */ #undef HAVE_TSEARCH /* Define to 1 if you have the header file. */ #undef HAVE_UNISTD_H /* Define to 1 if you have the `unsetenv' function. */ #undef HAVE_UNSETENV /* Define to 1 if the system has the type 'unsigned long long int'. */ #undef HAVE_UNSIGNED_LONG_LONG_INT /* Define to 1 if you have the `uselocale' function. */ #undef HAVE_USELOCALE /* Define to 1 if you have the `usleep' function. */ #undef HAVE_USLEEP /* Define if you have a global __progname variable */ #undef HAVE_VAR___PROGNAME /* Define to 1 if you have the `vasnprintf' function. */ #undef HAVE_VASNPRINTF /* Define to 1 if you have the `vsnprintf' function. */ #undef HAVE_VSNPRINTF /* Define to 1 if you have the header file. */ #undef HAVE_WCHAR_H /* Define if you have the 'wchar_t' type. */ #undef HAVE_WCHAR_T /* Define to 1 if you have the `wcrtomb' function. */ #undef HAVE_WCRTOMB /* Define to 1 if you have the `wcslen' function. */ #undef HAVE_WCSLEN /* Define to 1 if you have the `wcsnlen' function. */ #undef HAVE_WCSNLEN /* Define to 1 if you have the `wctob' function. */ #undef HAVE_WCTOB /* Define to 1 if you have the header file. */ #undef HAVE_WCTYPE_H /* Define to 1 if you have the `wcwidth' function. */ #undef HAVE_WCWIDTH /* Define to 1 if you have the header file. */ #undef HAVE_WINSOCK2_H /* Define if you have the 'wint_t' type. */ #undef HAVE_WINT_T /* Define to 1 if O_NOATIME works. */ #undef HAVE_WORKING_O_NOATIME /* Define to 1 if O_NOFOLLOW works. */ #undef HAVE_WORKING_O_NOFOLLOW /* Define to 1 if you have the header file. */ #undef HAVE_WS2TCPIP_H /* Define to 1 if you have the header file. */ #undef HAVE_XLOCALE_H /* Define to 1 if the system has the type `_Bool'. */ #undef HAVE__BOOL /* Define to 1 if you have the `_set_invalid_parameter_handler' function. */ #undef HAVE__SET_INVALID_PARAMETER_HANDLER /* Define to 1 if the compiler supports __builtin_expect, and to 2 if does. */ #undef HAVE___BUILTIN_EXPECT #ifndef HAVE___BUILTIN_EXPECT # define __builtin_expect(e, c) (e) #elif HAVE___BUILTIN_EXPECT == 2 # include #endif /* Define to 1 if you have the `__xpg_strerror_r' function. */ #undef HAVE___XPG_STRERROR_R /* In building, not usage */ #undef IN_GNUASTRO_BUILD /* Define as the bit index in the word where to find bit 0 of the exponent of 'long double'. */ #undef LDBL_EXPBIT0_BIT /* Define as the word index where to find the exponent of 'long double'. */ #undef LDBL_EXPBIT0_WORD /* Define as the bit index in the word where to find the sign of 'long double'. */ #undef LDBL_SIGNBIT_BIT /* Define as the word index where to find the sign of 'long double'. */ #undef LDBL_SIGNBIT_WORD /* Define to 1 if 'lstat' dereferences a symlink specified with a trailing slash. */ #undef LSTAT_FOLLOWS_SLASHED_SYMLINK /* Define to the sub-directory where libtool stores uninstalled libraries. */ #undef LT_OBJDIR /* If malloc(0) is != NULL, define this to 1. Otherwise define this to 0. */ #undef MALLOC_0_IS_NONNULL /* Define to a substitute value for mmap()'s MAP_ANONYMOUS flag. */ #undef MAP_ANONYMOUS /* Define if the mbrtowc function does not return (size_t) -2 for empty input. */ #undef MBRTOWC_EMPTY_INPUT_BUG /* Define if the mbrtowc function has the NULL pwc argument bug. */ #undef MBRTOWC_NULL_ARG1_BUG /* Define if the mbrtowc function has the NULL string argument bug. */ #undef MBRTOWC_NULL_ARG2_BUG /* Define if the mbrtowc function does not return 0 for a NUL character. */ #undef MBRTOWC_NUL_RETVAL_BUG /* Define if the mbrtowc function returns a wrong return value. */ #undef MBRTOWC_RETVAL_BUG /* Use GNU style printf and scanf. */ #ifndef __USE_MINGW_ANSI_STDIO # undef __USE_MINGW_ANSI_STDIO #endif /* Define to 1 if open() fails to recognize a trailing slash. */ #undef OPEN_TRAILING_SLASH_BUG /* Name of package */ #undef PACKAGE /* Define to the address where bug reports for this package should be sent. */ #undef PACKAGE_BUGREPORT /* Define to the full name of this package. */ #undef PACKAGE_NAME /* Define to the full name and version of this package. */ #undef PACKAGE_STRING /* Define to the one symbol short name of this package. */ #undef PACKAGE_TARNAME /* Define to the home page for this package. */ #undef PACKAGE_URL /* Define to the version of this package. */ #undef PACKAGE_VERSION /* Define if exists and defines unusable PRI* macros. */ #undef PRI_MACROS_BROKEN /* Define to the type that is the result of default argument promotions of type mode_t. */ #undef PROMOTED_MODE_T /* Define to necessary symbol if this constant uses a non-standard name on your system. */ #undef PTHREAD_CREATE_JOINABLE /* Define if the pthread_in_use() detection is hard. */ #undef PTHREAD_IN_USE_DETECTION_HARD /* Define to 1 if pthread_sigmask(), when it fails, returns -1 and sets errno. */ #undef PTHREAD_SIGMASK_FAILS_WITH_ERRNO /* Define to 1 if pthread_sigmask may return 0 and have no effect. */ #undef PTHREAD_SIGMASK_INEFFECTIVE /* Define to 1 if pthread_sigmask() unblocks signals incorrectly. */ #undef PTHREAD_SIGMASK_UNBLOCK_BUG /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'ptrdiff_t'. */ #undef PTRDIFF_T_SUFFIX /* Define to 1 if stat needs help when passed a file name with a trailing slash */ #undef REPLACE_FUNC_STAT_FILE /* Define if nl_langinfo exists but is overridden by gnulib. */ #undef REPLACE_NL_LANGINFO /* Define to 1 if strerror(0) does not return a message implying success. */ #undef REPLACE_STRERROR_0 /* Define if vasnprintf exists but is overridden by gnulib. */ #undef REPLACE_VASNPRINTF /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'sig_atomic_t'. */ #undef SIG_ATOMIC_T_SUFFIX /* The size of `long', as computed by sizeof. */ #undef SIZEOF_LONG /* The size of `size_t', as computed by sizeof. */ #undef SIZEOF_SIZE_T /* Define as the maximum value of type 'size_t', if the system doesn't define it. */ #ifndef SIZE_MAX # undef SIZE_MAX #endif /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'size_t'. */ #undef SIZE_T_SUFFIX /* If using the C implementation of alloca, define if you know the direction of stack growth for your system; otherwise it will be automatically deduced at runtime. STACK_DIRECTION > 0 => grows toward higher addresses STACK_DIRECTION < 0 => grows toward lower addresses STACK_DIRECTION = 0 => direction of growth unknown */ #undef STACK_DIRECTION /* Define to 1 if the `S_IS*' macros in do not work properly. */ #undef STAT_MACROS_BROKEN /* Define to 1 if you have the ANSI C header files. */ #undef STDC_HEADERS /* Define to 1 if strerror_r returns char *. */ #undef STRERROR_R_CHAR_P /* Define to 1 if the type of the st_atim member of a struct stat is struct timespec. */ #undef TYPEOF_STRUCT_STAT_ST_ATIM_IS_STRUCT_TIMESPEC /* User data dir. */ #undef USERCONFIG_DIR /* Define if the POSIX multithreading library can be used. */ #undef USE_POSIX_THREADS /* Define if references to the POSIX multithreading library should be made weak. */ #undef USE_POSIX_THREADS_WEAK /* Define if the GNU Pth multithreading library can be used. */ #undef USE_PTH_THREADS /* Define if references to the GNU Pth multithreading library should be made weak. */ #undef USE_PTH_THREADS_WEAK /* Define if the old Solaris multithreading library can be used. */ #undef USE_SOLARIS_THREADS /* Define if references to the old Solaris multithreading library should be made weak. */ #undef USE_SOLARIS_THREADS_WEAK /* Enable extensions on AIX 3, Interix. */ #ifndef _ALL_SOURCE # undef _ALL_SOURCE #endif /* Enable general extensions on macOS. */ #ifndef _DARWIN_C_SOURCE # undef _DARWIN_C_SOURCE #endif /* Enable GNU extensions on systems that have them. */ #ifndef _GNU_SOURCE # undef _GNU_SOURCE #endif /* Enable NetBSD extensions on NetBSD. */ #ifndef _NETBSD_SOURCE # undef _NETBSD_SOURCE #endif /* Enable OpenBSD extensions on NetBSD. */ #ifndef _OPENBSD_SOURCE # undef _OPENBSD_SOURCE #endif /* Enable threading extensions on Solaris. */ #ifndef _POSIX_PTHREAD_SEMANTICS # undef _POSIX_PTHREAD_SEMANTICS #endif /* Enable extensions specified by ISO/IEC TS 18661-5:2014. */ #ifndef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ # undef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-1:2014. */ #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ # undef __STDC_WANT_IEC_60559_BFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-2:2015. */ #ifndef __STDC_WANT_IEC_60559_DFP_EXT__ # undef __STDC_WANT_IEC_60559_DFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-4:2015. */ #ifndef __STDC_WANT_IEC_60559_FUNCS_EXT__ # undef __STDC_WANT_IEC_60559_FUNCS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-3:2015. */ #ifndef __STDC_WANT_IEC_60559_TYPES_EXT__ # undef __STDC_WANT_IEC_60559_TYPES_EXT__ #endif /* Enable extensions specified by ISO/IEC TR 24731-2:2010. */ #ifndef __STDC_WANT_LIB_EXT2__ # undef __STDC_WANT_LIB_EXT2__ #endif /* Enable extensions specified by ISO/IEC 24747:2009. */ #ifndef __STDC_WANT_MATH_SPEC_FUNCS__ # undef __STDC_WANT_MATH_SPEC_FUNCS__ #endif /* Enable extensions on HP NonStop. */ #ifndef _TANDEM_SOURCE # undef _TANDEM_SOURCE #endif /* Enable X/Open extensions if necessary. HP-UX 11.11 defines mbstate_t only if _XOPEN_SOURCE is defined to 500, regardless of whether compiling with -Ae or -D_HPUX_SOURCE=1. */ #ifndef _XOPEN_SOURCE # undef _XOPEN_SOURCE #endif /* Enable general extensions on Solaris. */ #ifndef __EXTENSIONS__ # undef __EXTENSIONS__ #endif /* Define if the native Windows multithreading API can be used. */ #undef USE_WINDOWS_THREADS /* Version number of package */ #undef VERSION /* Define to 1 if unsetenv returns void instead of int. */ #undef VOID_UNSETENV /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'wchar_t'. */ #undef WCHAR_T_SUFFIX /* Define if WSAStartup is needed. */ #undef WINDOWS_SOCKETS /* Define to l, ll, u, ul, ull, etc., as suitable for constants of type 'wint_t'. */ #undef WINT_T_SUFFIX /* Define WORDS_BIGENDIAN to 1 if your processor stores words with the most significant byte first (like Motorola and SPARC, unlike Intel). */ #if defined AC_APPLE_UNIVERSAL_BUILD # if defined __BIG_ENDIAN__ # define WORDS_BIGENDIAN 1 # endif #else # ifndef WORDS_BIGENDIAN # undef WORDS_BIGENDIAN # endif #endif /* Enable large inode numbers on Mac OS X 10.5. */ #undef _DARWIN_USE_64_BIT_INODE /* Number of bits in a file offset, on hosts where this is settable. */ #undef _FILE_OFFSET_BITS /* Define for large files, on AIX-style hosts. */ #undef _LARGE_FILES /* Define to 1 on Solaris. */ #undef _LCONV_C99 /* Define to 1 if on MINIX. */ #undef _MINIX /* Define to 1 to make NetBSD features available. MINIX 3 needs this. */ #undef _NETBSD_SOURCE /* The _Noreturn keyword of C11. */ #if ! (defined _Noreturn \ || (defined __STDC_VERSION__ && 201112 <= __STDC_VERSION__)) # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif defined _MSC_VER && 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif /* Define to 2 if the system does not provide POSIX.1 features except with this defined. */ #undef _POSIX_1_SOURCE /* Define to 1 in order to get the POSIX compatible declarations of socket functions. */ #undef _POSIX_PII_SOCKET /* Define to 1 if you need to in order for 'stat' and other things to work. */ #undef _POSIX_SOURCE /* Define if you want to include , so that it consistently overrides 's RE_DUP_MAX. */ #undef _REGEX_INCLUDE_LIMITS_H /* Define if you want regoff_t to be at least as wide POSIX requires. */ #undef _REGEX_LARGE_OFFSETS /* For standard stat data types on VMS. */ #undef _USE_STD_STAT /* Define to rpl_ if the getopt replacement functions and variables should be used. */ #undef __GETOPT_PREFIX /* Define to 1 if the system predates C++11. */ #undef __STDC_CONSTANT_MACROS /* Define to 1 if the system predates C++11. */ #undef __STDC_LIMIT_MACROS /* Define as a replacement for the ISO C99 __func__ variable. */ #undef __func__ /* Please see the Gnulib manual for how to use these macros. Suppress extern inline with HP-UX cc, as it appears to be broken; see . Suppress extern inline with Sun C in standards-conformance mode, as it mishandles inline functions that call each other. E.g., for 'inline void f (void) { } inline void g (void) { f (); }', c99 incorrectly complains 'reference to static identifier "f" in extern inline function'. This bug was observed with Sun C 5.12 SunOS_i386 2011/11/16. Suppress extern inline (with or without __attribute__ ((__gnu_inline__))) on configurations that mistakenly use 'static inline' to implement functions or macros in standard C headers like . For example, if isdigit is mistakenly implemented via a static inline function, a program containing an extern inline function that calls isdigit may not work since the C standard prohibits extern inline functions from calling static functions. This bug is known to occur on: OS X 10.8 and earlier; see: https://lists.gnu.org/r/bug-gnulib/2012-12/msg00023.html DragonFly; see http://muscles.dragonflybsd.org/bulk/bleeding-edge-potential/latest-per-pkg/ah-tty-0.3.12.log FreeBSD; see: https://lists.gnu.org/r/bug-gnulib/2014-07/msg00104.html OS X 10.9 has a macro __header_inline indicating the bug is fixed for C and for clang but remains for g++; see . Assume DragonFly and FreeBSD will be similar. */ #if (((defined __APPLE__ && defined __MACH__) \ || defined __DragonFly__ || defined __FreeBSD__) \ && (defined __header_inline \ ? (defined __cplusplus && defined __GNUC_STDC_INLINE__ \ && ! defined __clang__) \ : ((! defined _DONT_USE_CTYPE_INLINE_ \ && (defined __GNUC__ || defined __cplusplus)) \ || (defined _FORTIFY_SOURCE && 0 < _FORTIFY_SOURCE \ && defined __GNUC__ && ! defined __cplusplus)))) # define _GL_EXTERN_INLINE_STDHEADER_BUG #endif #if ((__GNUC__ \ ? defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ \ : (199901L <= __STDC_VERSION__ \ && !defined __HP_cc \ && !defined __PGI \ && !(defined __SUNPRO_C && __STDC__))) \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # define _GL_INLINE inline # define _GL_EXTERN_INLINE extern inline # define _GL_EXTERN_INLINE_IN_USE #elif (2 < __GNUC__ + (7 <= __GNUC_MINOR__) && !defined __STRICT_ANSI__ \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # if defined __GNUC_GNU_INLINE__ && __GNUC_GNU_INLINE__ /* __gnu_inline__ suppresses a GCC 4.2 diagnostic. */ # define _GL_INLINE extern inline __attribute__ ((__gnu_inline__)) # else # define _GL_INLINE extern inline # endif # define _GL_EXTERN_INLINE extern # define _GL_EXTERN_INLINE_IN_USE #else # define _GL_INLINE static _GL_UNUSED # define _GL_EXTERN_INLINE static _GL_UNUSED #endif /* In GCC 4.6 (inclusive) to 5.1 (exclusive), suppress bogus "no previous prototype for 'FOO'" and "no previous declaration for 'FOO'" diagnostics, when FOO is an inline function in the header; see and . */ #if __GNUC__ == 4 && 6 <= __GNUC_MINOR__ # if defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ # define _GL_INLINE_HEADER_CONST_PRAGMA # else # define _GL_INLINE_HEADER_CONST_PRAGMA \ _Pragma ("GCC diagnostic ignored \"-Wsuggest-attribute=const\"") # endif # define _GL_INLINE_HEADER_BEGIN \ _Pragma ("GCC diagnostic push") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-prototypes\"") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-declarations\"") \ _GL_INLINE_HEADER_CONST_PRAGMA # define _GL_INLINE_HEADER_END \ _Pragma ("GCC diagnostic pop") #else # define _GL_INLINE_HEADER_BEGIN # define _GL_INLINE_HEADER_END #endif /* Define to `int' if doesn't define. */ #undef gid_t /* Define to `__inline__' or `__inline' if that's what the C compiler calls it, or to nothing if 'inline' is not supported under any name. */ #ifndef __cplusplus #undef inline #endif /* Define to long or long long if and don't define. */ #undef intmax_t /* Work around a bug in Apple GCC 4.0.1 build 5465: In C99 mode, it supports the ISO C 99 semantics of 'extern inline' (unlike the GNU C semantics of earlier versions), but does not display it by setting __GNUC_STDC_INLINE__. __APPLE__ && __MACH__ test for Mac OS X. __APPLE_CC__ tests for the Apple compiler and its version. __STDC_VERSION__ tests for the C99 mode. */ #if defined __APPLE__ && defined __MACH__ && __APPLE_CC__ >= 5465 && !defined __cplusplus && __STDC_VERSION__ >= 199901L && !defined __GNUC_STDC_INLINE__ # define __GNUC_STDC_INLINE__ 1 #endif /* Define to rpl_malloc if the replacement function should be used. */ #undef malloc /* Define to a type if does not define. */ #undef mbstate_t /* Define to `int' if does not define. */ #undef mode_t /* Define to the type of st_nlink in struct stat, or a supertype. */ #undef nlink_t /* Define to `int' if does not define. */ #undef pid_t /* Define as the type of the result of subtracting two pointers, if the system doesn't define it. */ #undef ptrdiff_t /* Define to rpl_re_comp if the replacement should be used. */ #undef re_comp /* Define to rpl_re_compile_fastmap if the replacement should be used. */ #undef re_compile_fastmap /* Define to rpl_re_compile_pattern if the replacement should be used. */ #undef re_compile_pattern /* Define to rpl_re_exec if the replacement should be used. */ #undef re_exec /* Define to rpl_re_match if the replacement should be used. */ #undef re_match /* Define to rpl_re_match_2 if the replacement should be used. */ #undef re_match_2 /* Define to rpl_re_search if the replacement should be used. */ #undef re_search /* Define to rpl_re_search_2 if the replacement should be used. */ #undef re_search_2 /* Define to rpl_re_set_registers if the replacement should be used. */ #undef re_set_registers /* Define to rpl_re_set_syntax if the replacement should be used. */ #undef re_set_syntax /* Define to rpl_re_syntax_options if the replacement should be used. */ #undef re_syntax_options /* Define to rpl_regcomp if the replacement should be used. */ #undef regcomp /* Define to rpl_regerror if the replacement should be used. */ #undef regerror /* Define to rpl_regexec if the replacement should be used. */ #undef regexec /* Define to rpl_regfree if the replacement should be used. */ #undef regfree /* Define to the equivalent of the C99 'restrict' keyword, or to nothing if this is not supported. Do not define if restrict is supported directly. */ #undef restrict /* Work around a bug in Sun C++: it does not support _Restrict or __restrict__, even though the corresponding Sun C compiler ends up with "#define restrict _Restrict" or "#define restrict __restrict__" in the previous line. Perhaps some future version of Sun C++ will work with restrict; if so, hopefully it defines __RESTRICT like Sun C does. */ #if defined __SUNPRO_CC && !defined __RESTRICT # define _Restrict # define __restrict__ #endif /* Define to `unsigned int' if does not define. */ #undef size_t /* type to use in place of socklen_t if not defined */ #undef socklen_t /* Define as a signed type of the same size as size_t. */ #undef ssize_t /* Define to `int' if doesn't define. */ #undef uid_t /* Define as a marker that can be attached to declarations that might not be used. 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= @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ 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@GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINDOWS_STAT_INODES = @WINDOWS_STAT_INODES@ WINDOWS_STAT_TIMESPEC = @WINDOWS_STAT_TIMESPEC@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = @abs_top_srcdir@ ac_ct_AR = @ac_ct_AR@ ac_ct_CC = @ac_ct_CC@ ac_ct_CXX = @ac_ct_CXX@ ac_ct_DUMPBIN = @ac_ct_DUMPBIN@ am__include = @am__include@ am__leading_dot = @am__leading_dot@ am__quote = @am__quote@ am__tar = @am__tar@ am__untar = @am__untar@ ax_pthread_config = @ax_pthread_config@ bindir = @bindir@ build = @build@ build_alias = @build_alias@ build_cpu = @build_cpu@ build_os = @build_os@ build_vendor = @build_vendor@ builddir = @builddir@ datadir = @datadir@ datarootdir = @datarootdir@ docdir = @docdir@ dvidir = @dvidir@ exec_prefix = @exec_prefix@ gl_LIBOBJS = @gl_LIBOBJS@ 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The programs are run directory on the operating system's command-line enabling easy and efficient operation combined with other installed programs in shell scripts or Makefiles. The libraries are also usable in C and C++ programs. The full package comes with a comprehensive book or documentation in various formats (plain text, info, PDF and HTML): http://www.gnu.org/software/gnuastro/manual/ The Gnuastro book explains all the mathematical, physical and even historical concepts (when necessary) for effective usage of all the programs and libraries along with short examples for each program and full descriptions of all their options (in the "Invoking ProgramName' sections). There is also a separate chapter devoted to tutorials for effectively use Gnuastro combined with other software already available on your Unix-like operating system (see Chapter 2). If you have already installed gnuastro, you can read the full book by running the following command. You can go through the whole book by pressing the 'SPACE' key, and leave the Info environment at any time by pressing 'q' key. See the "Getting help" section below (in this file) or in the book for more. info gnuastro The programs released in version 0.2 are listed below followed by their executable name in parenthesis and a short description. This list is ordered alphabetically. In the book, they are grouped and ordered by context under categories/chapters. - Arithmetic (astarithmetic): For arithmetic operations on multiple (theoretically unlimited) number of datasets (images). It has a large and growing set of arithmetic, mathematical, and even statistical operators (for example +, -, *, /, sqrt, log, min, average, median). - BuildProgram (astbuildprog): Compile, link and run programs that depend on the Gnuastro library. BuildProgram will automatically link with the libraries that Gnuastro depends on, so there is no need to explicily mention them every time you are compiling a Gnuastro library dependent program. - ConvertType (astconvertt): Convert astronomical data files (FITS or IMH) to and from several other standard image and data formats, for example TXT, JPEG, EPS or PDF. - Convolve (astconvolve): Convolve (blur or smooth) data with a given kernel in spatial and frequency domain on multiple threads. Convolve can also do de-convolution to find the appropriate kernel to PSF-match two images. - CosmicCalculator (astconvolve): Do cosmological calculations, for example the luminosity distance, distance modulus, comoving volume and many more. - Crop (astcrop): Crop region(s) from an image and stitch several images if necessary. Inputs can be in pixel coordinates or world coordinates. - Header (astheader): Print and manipulate the header data of a FITS file. - Match (astmatch): Given two input catalogs, find the rows that match with each other within a given aperture (may be an ellipse). - MakeCatalog (astmkcatalog): Make catalog of labeled image (output of NoiseChisel). The catalogs are highly customizable and adding new calculations/columns is very streightforward. - MakeNoise (astmknoise): Make (add) noise to an image, with a large set of random number generators and any seed. - MakeProfiles (astmkprof): Make mock 2D profiles in an image. The central regions of radial profiles are made with a configurable 2D Monte Carlo integration. It can also build the profiles on an over-sampled image. - NoiseChisel (astnoisechisel): Detect and segment signal in noise. It uses a technique to detect very faint and diffuse, irregularly shaped signal in noise (galaxies in the sky), using thresholds that are below the Sky value (see arXiv:1505.01664). - Statistics (aststatistics): Get pixel statistics and save histogram and cumulative frequency plots. - Table (asttable): convert FITS binary and ASCII tables into other such tables, or print them on the command-line, or save them in a plain text file. Output columns can also be determined by number or regular expression matching of column names. - Warp (astwarp): Warp image to new pixel grid. Any projective transformation or Homography can be applied to the input images. All the programs share the same basic command-line user interface and a set of common options for the comfort of both the users and developers. Gnuastro is written to comply fully with the GNU coding standards so it integrates finely with the GNU/Linux operating system and Unix-like operating systems in general. This also enables astronomers to expect a fully familiar experience in the source code, building, installing and command line user interaction that they have seen in all the other GNU software that they use. Behind the scenes, Gnuastro comes with a very robust infra-structure enabling easy addition of new programs and new features to existing programs and a full chapter devoted to explaining how to develop most effectively (see the "Developing" chapter). Please join us in developing this comprehensive and low level set of tools for astronomical data manipulation and analysis. The copyright owner of Gnuastro is the Free Software Foundation to guarantee its freedom in the future, and not any particular astronomer or astronomical project, or astronomical institution, so please join us and feel free to use it in your research. Installing Gnuastro ------------------- The mandatory dependencies which are required to install Gnuastro from the tarball are listed below. See the "Dependencies" section of the book for their detailed installation guides and optional dependencies to enable extra features. If you have just cloned Gnuastro and want to install from the version controlled source, please read the 'README-hacking' file (not available in the tarball) or the "Bootstrapping dependencies" subsection of the manual before continuing. - GNU Scientific Library (GSL): https://www.gnu.org/software/gsl/ - CFITSIO: http://heasarc.gsfc.nasa.gov/fitsio/ - WCSLIB: http://www.atnf.csiro.au/people/mcalabre/WCS/ The most recent stable Gnuastro release can be downloaded from the following link. Please see the "Downloading the source" section of the Gnuastro book for a more complete discussion of your download options. http://ftp.gnu.org/gnu/gnuastro/gnuastro-latest.tar.gz Unpacking, configuring, building, checking and installing Gnuastro follows the standard GNU Build system as shown below. After the './configure' command, Gnuastro will print messages upon the successful completion of each step, giving further information and suggestions for the next steps. tar xf gnuastro-latest.tar.gz # Also works for `tar.lz' files cd gnuastro-0.1 ./configure make make check sudo make install See the "Build and install" section of the book for more information. Also, see the 'INSTALL' file which is distributed with this file for a standard (very comprehensive and general) review of the GNU build and install methods. The 'INSTALL' file is shared in many software packages, so reading it once in any package is enough to help you greatly customize your build of a very large collection of Free and Open Source (FOSS) software. Getting help ------------ To access the appropriate section of the Gnuastro book/documentation from your command-line (in the middle of your work, without distracting your self by having to move your hand off the keyboard), please run any of the following two commands. Note that you can leave the Info environment by pressing the key `q'. info ProgramName # For example 'info NoiseChisel' info astprogname # For example 'info astnoisechisel' The Info environment is great for easily reading of the complete documentation of many software packages, not just Gnuastro. It can greatly enhance your life/work in the Unix-like operating systems. If you are not familiar with it, please run the following command and read through it (it is short and only takes about an hour, so we strongly recommend it): info info To immediately get a short list of each programs's options and a short explanation of each, please run: astprogname --help # For example 'astnoisechisel --help' Ultimately you can send a mail to 'help-gnuastro@gnu.org' to get help in installing or using Gnuastro. Some Gnuastro developers and active users are subscribed to this list and are ready to help you in using these programs. Reporting bugs -------------- The most effective way to report bugs is explained in the "Report a bug" section of the documentation, after installation, you can read it by running (leave the Info environment by pressing the `q' key afterwards): info bug-gnuastro In short, you can send a mail to 'bug-gnuastro@gnu.org', or submit a report in the link below (the latter is recommended): https://savannah.gnu.org/support/?func=additem&group=gnuastro In any case, please be very descriptive and give the exact command that produced the bug, we will be able to solve it faster and more effectively if we can reproduce it after your first report. The list of previous bugs along with their status can be seen here https://savannah.gnu.org/bugs/?group=gnuastro Have a look in the link above to see if your problem has already been addressed. 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m4_include([bootstrapped/m4/vsnprintf.m4]) m4_include([bootstrapped/m4/warn-on-use.m4]) m4_include([bootstrapped/m4/wchar_h.m4]) m4_include([bootstrapped/m4/wchar_t.m4]) m4_include([bootstrapped/m4/wcrtomb.m4]) m4_include([bootstrapped/m4/wctob.m4]) m4_include([bootstrapped/m4/wctomb.m4]) m4_include([bootstrapped/m4/wctype_h.m4]) m4_include([bootstrapped/m4/wcwidth.m4]) m4_include([bootstrapped/m4/wint_t.m4]) m4_include([bootstrapped/m4/xsize.m4]) m4_include([bootstrapped/m4/yield.m4]) gnuastro-0.5/configure.ac0000644000175000017500000006762113215601241012436 00000000000000# Process this file with autoconf to produce a configure script. # # Hand written file: used as input into GNU Autotools (autoconf). # This is part of GNU Astronomy Utilities (gnuastro) package. # # We use some macros that are distributed as part of the GNU Autoconf # Archive here. 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If not, see . # Definitions: AC_PREREQ([2.69]) AC_INIT([GNU Astronomy Utilities], m4_esyscmd([bootstrapped/build-aux/git-version-gen \ .tarball-version --prefix "gnuastro_v"]), [bug-gnuastro@gnu.org], [gnuastro], [http://www.gnu.org/software/gnuastro/]) AC_CONFIG_AUX_DIR([bootstrapped/build-aux]) AM_INIT_AUTOMAKE([-Wall subdir-objects gnu]) AC_CONFIG_SRCDIR([lib/fits.c]) AC_CONFIG_HEADERS([config.h]) AC_CONFIG_MACRO_DIRS([bootstrapped/m4]) # Library version, see the GNU Libtool manual ("Library interface versions" # section for the exact definition of each) for GAL_CURRENT=3 GAL_REVISION=0 GAL_AGE=0 GAL_LT_VERSION="${GAL_CURRENT}:${GAL_REVISION}:${GAL_AGE}" AC_SUBST(GAL_LT_VERSION) # Checks for programs. : ${CFLAGS=""} : ${CXXFLAGS=""} AC_PROG_CC AC_PROG_CXX gl_EARLY AM_PROG_AR LT_INIT # This macro will let the libraries know that we are now in the Gnuastro # build system, not on the user's system. While we are building Gnuastro, # we have the important installation information in `config.h'. But in the # user's own programs, this information is defined in # `gnuastro/config.h'. With this macro, the installed headers can decide # if the latter should be included or not. Note that `gnuastro/config.h' # is only built at installation time and doesn't exist when building # Gnuastro. Therefore, this macro must not be defined in a user's program. AC_DEFINE([IN_GNUASTRO_BUILD], [1], [In building, not usage]) # Generic compiler flags for all sub-directories. CFLAGS="-Wall -O3 $CFLAGS" CXXFLAGS="-Wall -O3 $CXXFLAGS" LDFLAGS="-L\$(top_builddir)/lib $LDFLAGS" CPPFLAGS="-I\$(top_srcdir)/lib $CPPFLAGS" # Check for pthreads and add the appropriate compilation flags. AX_PTHREAD # comes from the GNU Autoconf Archive's ax_pthread.m4, see there for the # documentation. 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AC_CHECK_SIZEOF([size_t]) AC_SUBST(SIZEOF_SIZE_T, [$ac_cv_sizeof_size_t]) AC_DEFINE_UNQUOTED([GAL_CONFIG_SIZEOF_SIZE_T], [$ac_cv_sizeof_size_t], [On 32bit will be 4, on 64 bit, will be 8]) AC_CHECK_SIZEOF([long]) AC_SUBST(SIZEOF_LONG, [$ac_cv_sizeof_long]) AC_DEFINE_UNQUOTED([GAL_CONFIG_SIZEOF_LONG], [$ac_cv_sizeof_long], [On 32bit will be 4, on 64 bit, will be 8]) # By default we assume no warnings anywarnings=no # Remove any occurance of the current directory `./', `.', or the full # address of the current directory in PATH. The main problem is the # `libtool' executable which Gnuastro builds internally in the top build # directory. However, we also need to know if the system has libtool or # not. AC_MSG_CHECKING(if PATH contains current directory) oldPATH=$PATH currpwd=$(pwd) # The first call to SED will remove any occurance of the current directory: # `./', `.', or the full address. # # NOTE 1: We cannot simply remove all `.'s, because hidden directories # (like the `~/.local' that is suggested for local # installations) will also be altered. # # NOTE 2: An empty string in the list of strings (separated by `:') # means the current directory. This includes cases like: `::', # or a leading and trailing `:'. So after all the removals of # the current directory, we will remove all such cases. # # NOTE 3: The SED separator can be any character immediately after `s', # it doesn't just have to be the commonly used `/'. Since `$pwd' # will possibly contain many `/'s, it is much more easier to use # a differen separator (`|' in this call to SED). 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AC_SEARCH_LIBS(sqrt, m, [], [AC_MSG_ERROR([C math library not present, cannot continue.])]) AC_SEARCH_LIBS([cblas_sdsdot], [gslcblas], [], [AC_MSG_ERROR([GSL CBLAS not present, cannot continue.])]) AC_SEARCH_LIBS([gsl_integration_qng], [gsl], [], [AC_MSG_ERROR([GSL not found, cannot continue.])]) # Since version 0.42, if `libcurl' is installed, CFITSIO will link with it # and thus it will be necessary to explicitly link with libcurl also. If it # doesn't exist on the system, then CFITSIO won't link with it and there is # no problem for Gnuastro either. So there is no need to stop the configure # script if libcurl isn't found. AC_SEARCH_LIBS([curl_global_init], [curl], [], []) AC_SEARCH_LIBS([ffopen], [cfitsio], [], [AC_MSG_ERROR([CFITSIO not found, cannot continue.])]) AC_SEARCH_LIBS([wcspih], [wcs], [], [AC_MSG_ERROR([WCSLIB not found, cannot continue.])]) # These are secondary tests for more fine-grained control in libraries that # have already been checked. We don't need to add them to the LIBS # variable, so we are using AC_CHECK_LIB for these tests. # If the WCS library has the `wcslib_version' function. AC_CHECK_LIB([wcs], [wcslib_version], [has_wcslib_version=1], [has_wcslib_version=0], [-lcfitsio -lm]) AC_DEFINE_UNQUOTED([GAL_CONFIG_HAVE_WCSLIB_VERSION], [$has_wcslib_version], [WCSLIB comes with wcslib_version]) AC_SUBST(HAVE_WCSLIB_VERSION, [$has_wcslib_version]) # If the pthreads library has `pthread_barrier_wait'. AC_CHECK_LIB([pthread], [pthread_barrier_wait], [has_pthread_barrier=1], [has_pthread_barrier=0]) AC_DEFINE_UNQUOTED([GAL_CONFIG_HAVE_PTHREAD_BARRIER], [$has_pthread_barrier], [System has pthread_barrier]) AC_SUBST(HAVE_PTHREAD_BARRIER, [$has_pthread_barrier]) # Gnulib checks: gl_INIT # Gnulib checks for the proper name for the C99 equivalent `restrict' # keyword and puts it in the `ac_cv_c_restrict' variable. If none exists, # it will put a `no' inside of this variable. 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AS_IF([test "x$ac_cv_c_restrict" = "xno"], [gal_restrict_replace=], [gal_restrict_replace=$ac_cv_c_restrict]) AC_SUBST(RESTRICT_REPLACEMENT, [$gal_restrict_replace]) # To add the help2man: AC_CHECK_PROG(has_help2man, help2man, [yes], [no]) AM_CONDITIONAL([COND_HASHELP2MAN], [test "x$has_help2man" = "xyes"]) # Check libjpeg: AC_SEARCH_LIBS([jpeg_stdio_dest], [jpeg], [has_libjpeg=yes], [has_libjpeg=no]) AS_IF([test "x$has_libjpeg" = "xyes"], [AC_DEFINE([HAVE_LIBJPEG], [], [Has libjpeg])], [anywarnings=yes]) AM_CONDITIONAL([COND_HASLIBJPEG], [test "x$has_libjpeg" = "xyes"]) # Check libgit2: AC_SEARCH_LIBS([git_libgit2_init], [git2], [has_libgit2=1], [has_libgit2=0]) AC_DEFINE_UNQUOTED([GAL_CONFIG_HAVE_LIBGIT2], [$has_libgit2], [libgit2 is installed on the system]) AS_IF([test "x$has_libgit2" = "x1"], [], [anywarnings=yes]) AC_SUBST(HAVE_LIBGIT2, [$has_libgit2]) # Check the libtool executable on the system. Note that Gnuastro also ships # with a version of Libtool. We don't want Gnuastro's Libtool, here we want # to see if the system has libtool independent of Gnuastro so BuildProgram # can use it later. AC_CHECK_PROG(has_libtool, libtool, [yes], [no]) # If Libtool is present, make sure it is GNU Libtool AS_IF([test "x$has_libtool" = "xyes"], [ AC_MSG_CHECKING(if libtool executable is GNU) AS_IF( libtool --version 2> /dev/null | grep GNU 2>&1 > /dev/null, [has_gnulibtool=yes], [has_gnulibtool=no]) AC_MSG_RESULT( $has_gnulibtool )], [ has_gnulibtool=no ]) # When either the `libtool' executable isn't GNU or it doesn't exist, then # look for `glibtool'. AS_IF([test "x$has_gnulibtool" = "xyes"], [ gnulibtool_exec=libtool ], [ AC_CHECK_PROG(has_glibtool, glibtool, [yes], [no]) AS_IF( [test "x$has_glibtool" = "xyes"], [has_gnulibtool=yes; gnulibtool_exec=glibtool], [has_gnulibtool=no; anywarnings=yes] ) ]) # Write the test results in the Makefiles and `config.h'. AM_CONDITIONAL([COND_HASGNULIBTOOL], [test "x$has_gnulibtool" = "xyes"]) AC_DEFINE_UNQUOTED([GAL_CONFIG_GNULIBTOOL_EXEC], ["$gnulibtool_exec"], [The executable to call GNU Libtool]) # Check Ghostscript: "-dPDFFitPage" option to Ghostscript, used by # ConvertType to convert from EPS to PDF, has been introduced in # Ghostscript 9.10. Make sure we have at least that version. # # Below, only when Ghostscript exists, we check its version and only if its # version is larger than 9.10, does Gnuastro finally assume the existence # of Ghostscript. AX_COMPARE_VERSION comes from the GNU Autoconf Archive's # ax_compare_version.m4. AC_CHECK_PROG(has_ghostscript, gs, [yes], [no]) AS_IF([test "x$has_ghostscript" = "xyes"], [AC_MSG_CHECKING(Ghostscript version) gsversion=$(gs --version) AX_COMPARE_VERSION([9.10], [gt], [$gsversion], [has_ghostscript=no]) AC_MSG_RESULT( $gsversion )]) # Note: `has_ghostscript' can be set to `no' within the AS_IF above, so # `anywarnings' cannot be an [RUN-IF-FALSE] argument to the AS_IF above. AS_IF([test "x$has_ghostscript" = "xno"], [anywarnings=yes]) AM_CONDITIONAL([COND_HASGHOSTSCRIPT], [test "x$has_ghostscript" = "xyes"]) # Check if Gnulib tests should be done: AC_ARG_ENABLE([gnulibcheck], [AS_HELP_STRING([--enable-gnulibcheck], [In `make check', also test GNU Gnulib.])], [enable_gnulibcheck=yes], [enable_gnulibcheck=no]) AM_CONDITIONAL([COND_GNULIBCHECK], [test $enable_gnulibcheck = yes]) # Set the one general parameters: AC_DEFINE_UNQUOTED([CONF_POSTFIX], [".conf"], [Configuration file post fix.]) AC_DEFINE_UNQUOTED([USERCONFIG_DIR], [".local/etc"], [User data dir.]) AC_DEFINE_UNQUOTED([CONF_SHOWFMT], [" %-20s"], [Configuration file name format.]) # Read arguments about which programs to install. After checking if # the argument was actually called, remove any value the user might # have given by setting them to "yes" if they are not "no". 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AS_IF([test $ayes = true ], [ AS_IF([test $enable_arithmetic = notset], [enable_arithmetic=no]) AS_IF([test $enable_buildprog = notset], [enable_buildprog=no]) AS_IF([test $enable_convertt = notset], [enable_convertt=no]) AS_IF([test $enable_convolve = notset], [enable_convolve=no]) AS_IF([test $enable_cosmiccal = notset], [enable_cosmiccal=no]) AS_IF([test $enable_crop = notset], [enable_crop=no]) AS_IF([test $enable_fits = notset], [enable_fits=no]) AS_IF([test $enable_match = notset], [enable_match=no]) AS_IF([test $enable_mkcatalog = notset], [enable_mkcatalog=no]) AS_IF([test $enable_mknoise = notset], [enable_mknoise=no]) AS_IF([test $enable_mkprof = notset], [enable_mkprof=no]) AS_IF([test $enable_noisechisel = notset], [enable_noisechisel=no]) AS_IF([test $enable_statistics = notset], [enable_statistics=no]) AS_IF([test $enable_table = notset], [enable_table=no]) # AS_IF([test $enable_TEMPLATE = notset], [enable_TEMPLATE=no]) AS_IF([test $enable_warp = notset], [enable_warp=no]) ], [ AS_IF([test $enable_arithmetic = notset], [enable_arithmetic=yes]) AS_IF([test $enable_buildprog = notset], [enable_buildprog=yes]) AS_IF([test $enable_convertt = notset], [enable_convertt=yes]) AS_IF([test $enable_convolve = notset], [enable_convolve=yes]) AS_IF([test $enable_cosmiccal = notset], [enable_cosmiccal=yes]) AS_IF([test $enable_crop = notset], [enable_crop=yes]) AS_IF([test $enable_fits = notset], [enable_fits=yes]) AS_IF([test $enable_match = notset], [enable_match=yes]) AS_IF([test $enable_mkcatalog = notset], [enable_mkcatalog=yes]) AS_IF([test $enable_mknoise = notset], [enable_mknoise=yes]) AS_IF([test $enable_mkprof = notset], [enable_mkprof=yes]) AS_IF([test $enable_noisechisel = notset], [enable_noisechisel=yes]) AS_IF([test $enable_statistics = notset], [enable_statistics=yes]) AS_IF([test $enable_table = notset], [enable_table=yes]) # AS_IF([test $enable_TEMPLATE = notset], [enable_TEMPLATE=yes]) AS_IF([test $enable_warp = notset], [enable_warp=yes]) ] ) # BuildProgram depends on the presence of GNU Libtool, if it isn't present, # then don't build it. AS_IF([test "x$has_gnulibtool" = "xno"], [enable_buildprog=no]) # Make the enable_package values available for the Makefile: AM_CONDITIONAL([COND_ARITHMETIC], [test $enable_arithmetic = yes]) AM_CONDITIONAL([COND_BUILDPROG], [test $enable_buildprog = yes]) AM_CONDITIONAL([COND_CONVERTT], [test $enable_convertt = yes]) AM_CONDITIONAL([COND_CONVOLVE], [test $enable_convolve = yes]) AM_CONDITIONAL([COND_COSMICCAL], [test $enable_cosmiccal = yes]) AM_CONDITIONAL([COND_CROP], [test $enable_crop = yes]) AM_CONDITIONAL([COND_FITS], [test $enable_fits = yes]) AM_CONDITIONAL([COND_MATCH], [test $enable_match = yes]) AM_CONDITIONAL([COND_MKCATALOG], [test $enable_mkcatalog = yes]) AM_CONDITIONAL([COND_MKNOISE], [test $enable_mknoise = yes]) AM_CONDITIONAL([COND_MKPROF], [test $enable_mkprof = yes]) AM_CONDITIONAL([COND_NOISECHISEL], [test $enable_noisechisel = yes]) AM_CONDITIONAL([COND_STATISTICS], [test $enable_statistics = yes]) AM_CONDITIONAL([COND_TABLE], [test $enable_table = yes]) #AM_CONDITIONAL([COND_TEMPLATE], [test $enable_TEMPLATE = yes]) AM_CONDITIONAL([COND_WARP], [test $enable_warp = yes]) # Tell autoconf what to work on: TEMPLATE cannot be put and then # commented here like the cases above, so don't forget to add your new # utility name here. 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gltests_WITNESS NEXT_AS_FIRST_DIRECTIVE_WCHAR_H NEXT_WCHAR_H HAVE_FEATURES_H LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH_FALSE LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH_TRUE LIBUNISTRING_UNIWIDTH_H LIBUNISTRING_UNITYPES_H HAVE_UNISTD_H NEXT_AS_FIRST_DIRECTIVE_UNISTD_H NEXT_UNISTD_H GL_GENERATE_SYSEXITS_H_FALSE GL_GENERATE_SYSEXITS_H_TRUE SYSEXITS_H HAVE_SYSEXITS_H NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H NEXT_SYSEXITS_H WINDOWS_STAT_INODES WINDOWS_64_BIT_OFF_T NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H NEXT_SYS_TYPES_H HAVE_STRINGS_H NEXT_AS_FIRST_DIRECTIVE_STRINGS_H NEXT_STRINGS_H NEXT_AS_FIRST_DIRECTIVE_STRING_H NEXT_STRING_H HAVE_WINSOCK2_H REPLACE_IOCTL SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS SYS_IOCTL_H_HAVE_WINSOCK2_H GNULIB_IOCTL HAVE_DECL_STRNCASECMP HAVE_STRCASECMP HAVE_FFS GNULIB_FFS NEXT_AS_FIRST_DIRECTIVE_STDLIB_H NEXT_STDLIB_H NEXT_AS_FIRST_DIRECTIVE_STDIO_H NEXT_STDIO_H HAVE__BOOL GL_GENERATE_STDBOOL_H_FALSE GL_GENERATE_STDBOOL_H_TRUE STDBOOL_H GL_GENERATE_STDALIGN_H_FALSE GL_GENERATE_STDALIGN_H_TRUE STDALIGN_H HAVE_MSVC_INVALID_PARAMETER_HANDLER UNDEFINE_STRTOK_R REPLACE_STRSIGNAL REPLACE_STRERROR_R REPLACE_STRERROR REPLACE_STRTOK_R REPLACE_STRCASESTR REPLACE_STRSTR REPLACE_STRNLEN REPLACE_STRNDUP REPLACE_STRNCAT REPLACE_STRDUP REPLACE_STRCHRNUL REPLACE_STPNCPY REPLACE_MEMMEM REPLACE_MEMCHR HAVE_STRVERSCMP HAVE_DECL_STRSIGNAL HAVE_DECL_STRERROR_R HAVE_DECL_STRTOK_R HAVE_STRCASESTR HAVE_STRSEP HAVE_STRPBRK HAVE_DECL_STRNLEN HAVE_DECL_STRNDUP HAVE_DECL_STRDUP HAVE_STRCHRNUL HAVE_STPNCPY HAVE_STPCPY HAVE_RAWMEMCHR HAVE_DECL_MEMRCHR HAVE_MEMPCPY HAVE_DECL_MEMMEM HAVE_MEMCHR HAVE_FFSLL HAVE_FFSL HAVE_EXPLICIT_BZERO HAVE_MBSLEN GNULIB_STRVERSCMP GNULIB_STRSIGNAL GNULIB_STRERROR_R GNULIB_STRERROR GNULIB_MBSTOK_R GNULIB_MBSSEP GNULIB_MBSSPN GNULIB_MBSPBRK GNULIB_MBSCSPN GNULIB_MBSCASESTR GNULIB_MBSPCASECMP GNULIB_MBSNCASECMP GNULIB_MBSCASECMP GNULIB_MBSSTR GNULIB_MBSRCHR GNULIB_MBSCHR GNULIB_MBSNLEN GNULIB_MBSLEN GNULIB_STRTOK_R GNULIB_STRCASESTR GNULIB_STRSTR GNULIB_STRSEP GNULIB_STRPBRK GNULIB_STRNLEN GNULIB_STRNDUP GNULIB_STRNCAT GNULIB_STRDUP GNULIB_STRCHRNUL GNULIB_STPNCPY GNULIB_STPCPY GNULIB_RAWMEMCHR GNULIB_MEMRCHR GNULIB_MEMPCPY GNULIB_MEMMEM GNULIB_MEMCHR GNULIB_FFSLL GNULIB_FFSL GNULIB_EXPLICIT_BZERO LOCALE_FR_UTF8 LOCALE_ZH_CN LOCALE_JA NEXT_AS_FIRST_DIRECTIVE_MATH_H NEXT_MATH_H REPLACE_TRUNCL REPLACE_TRUNCF REPLACE_TRUNC REPLACE_TANHF REPLACE_TANF REPLACE_SQRTL REPLACE_SQRTF REPLACE_SINHF REPLACE_SINF REPLACE_SIGNBIT_USING_GCC REPLACE_SIGNBIT REPLACE_ROUNDL REPLACE_ROUNDF REPLACE_ROUND REPLACE_REMAINDERL REPLACE_REMAINDERF REPLACE_REMAINDER REPLACE_NAN REPLACE_MODFL REPLACE_MODFF REPLACE_MODF REPLACE_LOGBL REPLACE_LOGBF REPLACE_LOGB REPLACE_LOG2L REPLACE_LOG2F REPLACE_LOG2 REPLACE_LOG1PL REPLACE_LOG1PF REPLACE_LOG1P REPLACE_LOG10L REPLACE_LOG10F REPLACE_LOG10 REPLACE_LOGL REPLACE_LOGF REPLACE_LOG REPLACE_LDEXPL REPLACE_ISNAN REPLACE_ISINF REPLACE_ISFINITE REPLACE_ILOGBL REPLACE_ILOGBF REPLACE_ILOGB REPLACE_HYPOTL REPLACE_HYPOTF REPLACE_HYPOT REPLACE_HUGE_VAL REPLACE_FREXPL REPLACE_FREXP REPLACE_FREXPF REPLACE_FMODL REPLACE_FMODF REPLACE_FMOD REPLACE_FMAL REPLACE_FMAF REPLACE_FMA REPLACE_FLOORL REPLACE_FLOORF REPLACE_FLOOR REPLACE_FABSL REPLACE_EXP2L REPLACE_EXP2 REPLACE_EXPM1F REPLACE_EXPM1 REPLACE_EXPF REPLACE_COSHF REPLACE_COSF REPLACE_CEILL REPLACE_CEILF REPLACE_CEIL REPLACE_CBRTL REPLACE_CBRTF REPLACE_ATAN2F REPLACE_ATANF REPLACE_ASINF REPLACE_ACOSF HAVE_DECL_TRUNCL HAVE_DECL_TRUNCF HAVE_DECL_TRUNC HAVE_DECL_TANL HAVE_DECL_SQRTL HAVE_DECL_SINL HAVE_DECL_ROUNDL HAVE_DECL_ROUNDF HAVE_DECL_ROUND HAVE_DECL_RINTF HAVE_DECL_REMAINDERL HAVE_DECL_REMAINDER HAVE_DECL_LOGB HAVE_DECL_LOG2L HAVE_DECL_LOG2F HAVE_DECL_LOG2 HAVE_DECL_LOG10L HAVE_DECL_LOGL HAVE_DECL_LDEXPL HAVE_DECL_FREXPL HAVE_DECL_FLOORL HAVE_DECL_FLOORF HAVE_DECL_EXPM1L HAVE_DECL_EXP2L HAVE_DECL_EXP2F HAVE_DECL_EXP2 HAVE_DECL_EXPL HAVE_DECL_COSL HAVE_DECL_COPYSIGNF HAVE_DECL_CEILL HAVE_DECL_CEILF HAVE_DECL_CBRTL HAVE_DECL_CBRTF HAVE_DECL_ATANL HAVE_DECL_ASINL HAVE_DECL_ACOSL HAVE_TANHF HAVE_TANL HAVE_TANF HAVE_SQRTL HAVE_SQRTF HAVE_SINHF HAVE_SINL HAVE_SINF HAVE_RINTL HAVE_RINT HAVE_REMAINDERF HAVE_REMAINDER HAVE_POWF HAVE_MODFL HAVE_MODFF HAVE_LOGBL HAVE_LOGBF HAVE_LOG1PL HAVE_LOG1PF HAVE_LOG1P HAVE_LOG10L HAVE_LOG10F HAVE_LOGL HAVE_LOGF HAVE_LDEXPF HAVE_ISNANL HAVE_ISNAND HAVE_ISNANF HAVE_ILOGBL HAVE_ILOGBF HAVE_ILOGB HAVE_HYPOTL HAVE_HYPOTF HAVE_FREXPF HAVE_FMODL HAVE_FMODF HAVE_FMAL HAVE_FMAF HAVE_FMA HAVE_FABSL HAVE_FABSF HAVE_EXPM1F HAVE_EXPM1 HAVE_EXPL HAVE_EXPF HAVE_COSHF HAVE_COSL HAVE_COSF HAVE_COPYSIGNL HAVE_COPYSIGN HAVE_CBRTL HAVE_CBRTF HAVE_CBRT HAVE_ATAN2F HAVE_ATANL HAVE_ATANF HAVE_ASINL HAVE_ASINF HAVE_ACOSL HAVE_ACOSF GNULIB_TRUNCL GNULIB_TRUNCF GNULIB_TRUNC GNULIB_TANHF GNULIB_TANL GNULIB_TANF GNULIB_SQRTL GNULIB_SQRTF GNULIB_SINHF GNULIB_SINL GNULIB_SINF GNULIB_SIGNBIT GNULIB_ROUNDL GNULIB_ROUNDF GNULIB_ROUND GNULIB_RINTL GNULIB_RINTF GNULIB_RINT GNULIB_REMAINDERL GNULIB_REMAINDERF GNULIB_REMAINDER GNULIB_POWF GNULIB_MODFL GNULIB_MODFF GNULIB_MODF GNULIB_LOGBL GNULIB_LOGBF GNULIB_LOGB GNULIB_LOG2L GNULIB_LOG2F GNULIB_LOG2 GNULIB_LOG1PL GNULIB_LOG1PF GNULIB_LOG1P GNULIB_LOG10L GNULIB_LOG10F GNULIB_LOG10 GNULIB_LOGL GNULIB_LOGF GNULIB_LOG GNULIB_LDEXPL GNULIB_LDEXPF GNULIB_ISNANL GNULIB_ISNAND GNULIB_ISNANF GNULIB_ISNAN GNULIB_ISINF GNULIB_ISFINITE GNULIB_ILOGBL GNULIB_ILOGBF GNULIB_ILOGB GNULIB_HYPOTL GNULIB_HYPOTF GNULIB_HYPOT GNULIB_FREXPL GNULIB_FREXP GNULIB_FREXPF GNULIB_FMODL GNULIB_FMODF GNULIB_FMOD GNULIB_FMAL GNULIB_FMAF GNULIB_FMA GNULIB_FLOORL GNULIB_FLOORF GNULIB_FLOOR GNULIB_FABSL GNULIB_FABSF GNULIB_EXPM1L GNULIB_EXPM1F GNULIB_EXPM1 GNULIB_EXP2L GNULIB_EXP2F GNULIB_EXP2 GNULIB_EXPL GNULIB_EXPF GNULIB_COSHF GNULIB_COSL GNULIB_COSF GNULIB_COPYSIGNL GNULIB_COPYSIGNF GNULIB_COPYSIGN GNULIB_CEILL GNULIB_CEILF GNULIB_CEIL GNULIB_CBRTL GNULIB_CBRTF GNULIB_CBRT GNULIB_ATAN2F GNULIB_ATANL GNULIB_ATANF GNULIB_ASINL GNULIB_ASINF GNULIB_ACOSL GNULIB_ACOSF REPLACE_WCTOMB REPLACE_UNSETENV REPLACE_STRTOD REPLACE_SETENV REPLACE_REALPATH REPLACE_REALLOC REPLACE_RANDOM_R REPLACE_QSORT_R REPLACE_PUTENV REPLACE_PTSNAME_R REPLACE_PTSNAME REPLACE_MKSTEMP REPLACE_MBTOWC REPLACE_MALLOC REPLACE_CANONICALIZE_FILE_NAME REPLACE_CALLOC HAVE_DECL_UNSETENV HAVE_UNLOCKPT HAVE_SYS_LOADAVG_H HAVE_STRUCT_RANDOM_DATA HAVE_STRTOULL HAVE_STRTOLL HAVE_STRTOD HAVE_DECL_SETSTATE HAVE_DECL_SETENV HAVE_SETENV HAVE_SECURE_GETENV HAVE_RPMATCH HAVE_REALPATH HAVE_REALLOCARRAY HAVE_RANDOM_R HAVE_RANDOM_H HAVE_RANDOM HAVE_QSORT_R HAVE_PTSNAME_R HAVE_PTSNAME HAVE_POSIX_OPENPT HAVE_MKSTEMPS HAVE_MKSTEMP HAVE_MKOSTEMPS HAVE_MKOSTEMP HAVE_MKDTEMP HAVE_DECL_INITSTATE HAVE_GRANTPT HAVE_GETSUBOPT HAVE_DECL_GETLOADAVG HAVE_CANONICALIZE_FILE_NAME HAVE_ATOLL HAVE__EXIT GNULIB_WCTOMB GNULIB_UNSETENV GNULIB_UNLOCKPT GNULIB_SYSTEM_POSIX GNULIB_STRTOULL GNULIB_STRTOLL GNULIB_STRTOD GNULIB_SETENV GNULIB_SECURE_GETENV GNULIB_RPMATCH GNULIB_REALPATH GNULIB_REALLOC_POSIX GNULIB_REALLOCARRAY GNULIB_RANDOM_R GNULIB_RANDOM GNULIB_QSORT_R GNULIB_PUTENV GNULIB_PTSNAME_R GNULIB_PTSNAME GNULIB_POSIX_OPENPT GNULIB_MKSTEMPS GNULIB_MKSTEMP GNULIB_MKOSTEMPS GNULIB_MKOSTEMP GNULIB_MKDTEMP GNULIB_MBTOWC GNULIB_MALLOC_POSIX GNULIB_GRANTPT GNULIB_GETSUBOPT GNULIB_GETLOADAVG GNULIB_CANONICALIZE_FILE_NAME GNULIB_CALLOC_POSIX GNULIB_ATOLL GNULIB__EXIT LTLIBMULTITHREAD LIBMULTITHREAD LTLIBTHREAD LIBTHREAD LIBPTH_PREFIX LTLIBPTH LIBPTH NEXT_AS_FIRST_DIRECTIVE_LOCALE_H NEXT_LOCALE_H HAVE_XLOCALE_H NEXT_AS_FIRST_DIRECTIVE_STDDEF_H NEXT_STDDEF_H GL_GENERATE_STDDEF_H_FALSE GL_GENERATE_STDDEF_H_TRUE STDDEF_H HAVE_WCHAR_T HAVE_MAX_ALIGN_T REPLACE_NULL REPLACE_STRUCT_LCONV REPLACE_DUPLOCALE REPLACE_SETLOCALE REPLACE_LOCALECONV HAVE_DUPLOCALE GNULIB_DUPLOCALE GNULIB_SETLOCALE GNULIB_LOCALECONV LOCALCHARSET_TESTS_ENVIRONMENT GLIBC21 HAVE_LANGINFO_YESEXPR HAVE_LANGINFO_ERA HAVE_LANGINFO_T_FMT_AMPM HAVE_LANGINFO_CODESET HAVE_LANGINFO_H NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H NEXT_LANGINFO_H REPLACE_NL_LANGINFO HAVE_NL_LANGINFO GNULIB_NL_LANGINFO REPLACE_TOWLOWER REPLACE_ISWCNTRL HAVE_WCTYPE_H NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H NEXT_WCTYPE_H HAVE_CRTDEFS_H HAVE_WINT_T HAVE_ISWCNTRL REPLACE_ISWBLANK HAVE_WCTRANS_T HAVE_WCTYPE_T HAVE_ISWBLANK GNULIB_TOWCTRANS GNULIB_WCTRANS GNULIB_ISWCTYPE GNULIB_WCTYPE GNULIB_ISWBLANK NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H NEXT_INTTYPES_H UINT64_MAX_EQ_ULONG_MAX UINT32_MAX_LT_UINTMAX_MAX PRIPTR_PREFIX PRI_MACROS_BROKEN INT64_MAX_EQ_LONG_MAX INT32_MAX_LT_INTMAX_MAX REPLACE_STRTOUMAX REPLACE_STRTOIMAX HAVE_DECL_STRTOUMAX HAVE_DECL_STRTOIMAX HAVE_DECL_IMAXDIV HAVE_DECL_IMAXABS GNULIB_STRTOUMAX GNULIB_STRTOIMAX GNULIB_IMAXDIV GNULIB_IMAXABS GL_GENERATE_STDINT_H_FALSE GL_GENERATE_STDINT_H_TRUE STDINT_H HAVE_SYS_INTTYPES_H HAVE_SYS_BITYPES_H HAVE_C99_STDINT_H WINT_T_SUFFIX WCHAR_T_SUFFIX SIG_ATOMIC_T_SUFFIX SIZE_T_SUFFIX PTRDIFF_T_SUFFIX HAVE_SIGNED_WINT_T HAVE_SIGNED_WCHAR_T HAVE_SIGNED_SIG_ATOMIC_T BITSIZEOF_WINT_T BITSIZEOF_WCHAR_T BITSIZEOF_SIG_ATOMIC_T BITSIZEOF_SIZE_T BITSIZEOF_PTRDIFF_T APPLE_UNIVERSAL_BUILD HAVE_STDINT_H NEXT_AS_FIRST_DIRECTIVE_STDINT_H NEXT_STDINT_H HAVE_SYS_TYPES_H HAVE_INTTYPES_H HAVE_WCHAR_H HAVE_UNSIGNED_LONG_LONG_INT HAVE_LONG_LONG_INT GNULIB_OVERRIDES_WINT_T GL_GENERATE_LIMITS_H_FALSE GL_GENERATE_LIMITS_H_TRUE LIMITS_H NEXT_AS_FIRST_DIRECTIVE_LIMITS_H NEXT_LIMITS_H HOST_CPU_C_ABI HOST_CPU LTLIBINTL LIBINTL GNULIB_GL_UNISTD_H_GETOPT GETOPT_CDEFS_H GETOPT_H HAVE_SYS_CDEFS_H HAVE_GETOPT_H NEXT_AS_FIRST_DIRECTIVE_GETOPT_H NEXT_GETOPT_H UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS UNISTD_H_HAVE_WINSOCK2_H REPLACE_WRITE REPLACE_USLEEP REPLACE_UNLINKAT REPLACE_UNLINK REPLACE_TTYNAME_R REPLACE_TRUNCATE REPLACE_SYMLINKAT REPLACE_SYMLINK REPLACE_SLEEP REPLACE_RMDIR REPLACE_READLINKAT REPLACE_READLINK REPLACE_READ REPLACE_PWRITE REPLACE_PREAD REPLACE_LSEEK REPLACE_LINKAT REPLACE_LINK REPLACE_LCHOWN REPLACE_ISATTY REPLACE_GETPAGESIZE REPLACE_GETGROUPS REPLACE_GETLOGIN_R REPLACE_GETDTABLESIZE REPLACE_GETDOMAINNAME REPLACE_GETCWD REPLACE_FTRUNCATE REPLACE_FCHOWNAT REPLACE_FACCESSAT REPLACE_DUP2 REPLACE_DUP REPLACE_CLOSE REPLACE_CHOWN HAVE_SYS_PARAM_H HAVE_OS_H HAVE_DECL_TTYNAME_R HAVE_DECL_SETHOSTNAME HAVE_DECL_GETUSERSHELL HAVE_DECL_GETPAGESIZE HAVE_DECL_GETLOGIN_R HAVE_DECL_GETLOGIN HAVE_DECL_GETDOMAINNAME HAVE_DECL_FDATASYNC HAVE_DECL_FCHDIR HAVE_DECL_ENVIRON HAVE_USLEEP HAVE_UNLINKAT HAVE_TRUNCATE HAVE_SYMLINKAT HAVE_SYMLINK HAVE_SLEEP HAVE_SETHOSTNAME HAVE_READLINKAT HAVE_READLINK HAVE_PWRITE HAVE_PREAD HAVE_PIPE2 HAVE_PIPE HAVE_LINKAT HAVE_LINK HAVE_LCHOWN HAVE_GROUP_MEMBER HAVE_GETPAGESIZE HAVE_GETLOGIN HAVE_GETHOSTNAME HAVE_GETGROUPS HAVE_GETDTABLESIZE HAVE_FTRUNCATE HAVE_FSYNC HAVE_FDATASYNC HAVE_FCHOWNAT HAVE_FCHDIR HAVE_FACCESSAT HAVE_EUIDACCESS HAVE_DUP3 HAVE_DUP2 HAVE_CHOWN GNULIB_WRITE GNULIB_USLEEP GNULIB_UNLINKAT GNULIB_UNLINK GNULIB_UNISTD_H_SIGPIPE GNULIB_UNISTD_H_NONBLOCKING GNULIB_TTYNAME_R GNULIB_TRUNCATE GNULIB_SYMLINKAT GNULIB_SYMLINK GNULIB_SLEEP GNULIB_SETHOSTNAME GNULIB_RMDIR GNULIB_READLINKAT GNULIB_READLINK GNULIB_READ GNULIB_PWRITE GNULIB_PREAD GNULIB_PIPE2 GNULIB_PIPE GNULIB_LSEEK GNULIB_LINKAT GNULIB_LINK GNULIB_LCHOWN GNULIB_ISATTY GNULIB_GROUP_MEMBER GNULIB_GETUSERSHELL GNULIB_GETPAGESIZE GNULIB_GETLOGIN_R GNULIB_GETLOGIN GNULIB_GETHOSTNAME GNULIB_GETGROUPS GNULIB_GETDTABLESIZE GNULIB_GETDOMAINNAME GNULIB_GETCWD GNULIB_FTRUNCATE GNULIB_FSYNC GNULIB_FDATASYNC GNULIB_FCHOWNAT GNULIB_FCHDIR GNULIB_FACCESSAT GNULIB_EUIDACCESS GNULIB_ENVIRON GNULIB_DUP3 GNULIB_DUP2 GNULIB_DUP GNULIB_CLOSE GNULIB_CHOWN GNULIB_CHDIR REPLACE_VSPRINTF REPLACE_VSNPRINTF REPLACE_VPRINTF REPLACE_VFPRINTF REPLACE_VDPRINTF REPLACE_VASPRINTF REPLACE_TMPFILE REPLACE_STDIO_WRITE_FUNCS REPLACE_STDIO_READ_FUNCS REPLACE_SPRINTF REPLACE_SNPRINTF REPLACE_RENAMEAT REPLACE_RENAME REPLACE_REMOVE REPLACE_PRINTF REPLACE_POPEN REPLACE_PERROR REPLACE_OBSTACK_PRINTF REPLACE_GETLINE REPLACE_GETDELIM REPLACE_FTELLO REPLACE_FTELL REPLACE_FSEEKO REPLACE_FSEEK REPLACE_FREOPEN REPLACE_FPURGE REPLACE_FPRINTF REPLACE_FOPEN REPLACE_FFLUSH REPLACE_FDOPEN REPLACE_FCLOSE REPLACE_DPRINTF HAVE_VDPRINTF HAVE_VASPRINTF HAVE_RENAMEAT HAVE_POPEN HAVE_PCLOSE HAVE_FTELLO HAVE_FSEEKO HAVE_DPRINTF HAVE_DECL_VSNPRINTF HAVE_DECL_SNPRINTF HAVE_DECL_OBSTACK_PRINTF HAVE_DECL_GETLINE HAVE_DECL_GETDELIM HAVE_DECL_FTELLO HAVE_DECL_FSEEKO HAVE_DECL_FPURGE GNULIB_VSPRINTF_POSIX GNULIB_VSNPRINTF GNULIB_VPRINTF_POSIX GNULIB_VPRINTF GNULIB_VFPRINTF_POSIX GNULIB_VFPRINTF GNULIB_VDPRINTF GNULIB_VSCANF GNULIB_VFSCANF GNULIB_VASPRINTF GNULIB_TMPFILE GNULIB_STDIO_H_SIGPIPE GNULIB_STDIO_H_NONBLOCKING GNULIB_SPRINTF_POSIX GNULIB_SNPRINTF GNULIB_SCANF GNULIB_RENAMEAT GNULIB_RENAME GNULIB_REMOVE GNULIB_PUTS GNULIB_PUTCHAR GNULIB_PUTC GNULIB_PRINTF_POSIX GNULIB_PRINTF GNULIB_POPEN GNULIB_PERROR GNULIB_PCLOSE GNULIB_OBSTACK_PRINTF_POSIX GNULIB_OBSTACK_PRINTF GNULIB_GETLINE GNULIB_GETDELIM GNULIB_GETCHAR GNULIB_GETC GNULIB_FWRITE GNULIB_FTELLO GNULIB_FTELL GNULIB_FSEEKO GNULIB_FSEEK GNULIB_FSCANF GNULIB_FREOPEN GNULIB_FREAD GNULIB_FPUTS GNULIB_FPUTC GNULIB_FPURGE GNULIB_FPRINTF_POSIX GNULIB_FPRINTF GNULIB_FOPEN GNULIB_FGETS GNULIB_FGETC GNULIB_FFLUSH GNULIB_FDOPEN GNULIB_FCLOSE GNULIB_DPRINTF REPLACE_ITOLD GL_GENERATE_FLOAT_H_FALSE GL_GENERATE_FLOAT_H_TRUE FLOAT_H NEXT_AS_FIRST_DIRECTIVE_FLOAT_H NEXT_FLOAT_H EOVERFLOW_VALUE EOVERFLOW_HIDDEN ENOLINK_VALUE ENOLINK_HIDDEN EMULTIHOP_VALUE EMULTIHOP_HIDDEN GL_GENERATE_ERRNO_H_FALSE GL_GENERATE_ERRNO_H_TRUE ERRNO_H NEXT_AS_FIRST_DIRECTIVE_ERRNO_H NEXT_ERRNO_H PRAGMA_COLUMNS PRAGMA_SYSTEM_HEADER INCLUDE_NEXT_AS_FIRST_DIRECTIVE INCLUDE_NEXT pkglibexecdir runstatedir lispdir LOCALE_FR REPLACE_WCSFTIME REPLACE_WCSWIDTH REPLACE_WCWIDTH REPLACE_WCSNRTOMBS REPLACE_WCSRTOMBS REPLACE_WCRTOMB REPLACE_MBSNRTOWCS REPLACE_MBSRTOWCS REPLACE_MBRLEN REPLACE_MBRTOWC REPLACE_MBSINIT REPLACE_WCTOB REPLACE_BTOWC REPLACE_MBSTATE_T HAVE_DECL_WCWIDTH HAVE_DECL_WCTOB HAVE_WCSFTIME HAVE_WCSWIDTH HAVE_WCSTOK HAVE_WCSSTR HAVE_WCSPBRK HAVE_WCSSPN HAVE_WCSCSPN HAVE_WCSRCHR HAVE_WCSCHR HAVE_WCSDUP HAVE_WCSXFRM HAVE_WCSCOLL HAVE_WCSNCASECMP HAVE_WCSCASECMP HAVE_WCSNCMP HAVE_WCSCMP HAVE_WCSNCAT HAVE_WCSCAT HAVE_WCPNCPY HAVE_WCSNCPY HAVE_WCPCPY HAVE_WCSCPY HAVE_WCSNLEN HAVE_WCSLEN HAVE_WMEMSET HAVE_WMEMMOVE HAVE_WMEMCPY HAVE_WMEMCMP HAVE_WMEMCHR HAVE_WCSNRTOMBS HAVE_WCSRTOMBS HAVE_WCRTOMB HAVE_MBSNRTOWCS HAVE_MBSRTOWCS HAVE_MBRLEN HAVE_MBRTOWC HAVE_MBSINIT HAVE_BTOWC GNULIB_WCSFTIME GNULIB_WCSWIDTH GNULIB_WCSTOK GNULIB_WCSSTR GNULIB_WCSPBRK GNULIB_WCSSPN GNULIB_WCSCSPN GNULIB_WCSRCHR GNULIB_WCSCHR GNULIB_WCSDUP GNULIB_WCSXFRM GNULIB_WCSCOLL GNULIB_WCSNCASECMP GNULIB_WCSCASECMP GNULIB_WCSNCMP GNULIB_WCSCMP GNULIB_WCSNCAT GNULIB_WCSCAT GNULIB_WCPNCPY GNULIB_WCSNCPY GNULIB_WCPCPY GNULIB_WCSCPY GNULIB_WCSNLEN GNULIB_WCSLEN GNULIB_WMEMSET GNULIB_WMEMMOVE GNULIB_WMEMCPY GNULIB_WMEMCMP GNULIB_WMEMCHR GNULIB_WCWIDTH GNULIB_WCSNRTOMBS GNULIB_WCSRTOMBS GNULIB_WCRTOMB GNULIB_MBSNRTOWCS GNULIB_MBSRTOWCS GNULIB_MBRLEN GNULIB_MBRTOWC GNULIB_MBSINIT GNULIB_WCTOB GNULIB_BTOWC GL_GENERATE_ALLOCA_H_FALSE GL_GENERATE_ALLOCA_H_TRUE ALLOCA_H ALLOCA LTALLOCA GL_COND_LIBTOOL_FALSE GL_COND_LIBTOOL_TRUE HAVE_PTHREAD_BARRIER HAVE_WCSLIB_VERSION SIZEOF_LONG SIZEOF_SIZE_T LIBOBJS PTHREAD_CFLAGS PTHREAD_LIBS PTHREAD_CC ax_pthread_config CXXCPP LT_SYS_LIBRARY_PATH OTOOL64 OTOOL LIPO NMEDIT DSYMUTIL MANIFEST_TOOL DLLTOOL OBJDUMP LN_S NM ac_ct_DUMPBIN DUMPBIN LD FGREP SED LIBTOOL host_os host_vendor host_cpu host build_os build_vendor build_cpu build RANLIB ARFLAGS ac_ct_AR AR EGREP GREP CPP am__fastdepCXX_FALSE am__fastdepCXX_TRUE CXXDEPMODE ac_ct_CXX CXXFLAGS CXX am__fastdepCC_FALSE am__fastdepCC_TRUE CCDEPMODE am__nodep AMDEPBACKSLASH AMDEP_FALSE AMDEP_TRUE am__quote am__include DEPDIR OBJEXT EXEEXT ac_ct_CC CPPFLAGS LDFLAGS CFLAGS CC GAL_LT_VERSION AM_BACKSLASH AM_DEFAULT_VERBOSITY AM_DEFAULT_V AM_V am__untar am__tar AMTAR am__leading_dot SET_MAKE AWK mkdir_p MKDIR_P INSTALL_STRIP_PROGRAM STRIP install_sh MAKEINFO AUTOHEADER AUTOMAKE AUTOCONF ACLOCAL VERSION PACKAGE CYGPATH_W am__isrc INSTALL_DATA INSTALL_SCRIPT INSTALL_PROGRAM target_alias host_alias build_alias LIBS ECHO_T ECHO_N ECHO_C DEFS mandir localedir libdir psdir pdfdir dvidir htmldir infodir docdir oldincludedir includedir localstatedir sharedstatedir sysconfdir datadir datarootdir libexecdir sbindir bindir program_transform_name prefix exec_prefix PACKAGE_URL PACKAGE_BUGREPORT PACKAGE_STRING PACKAGE_VERSION PACKAGE_TARNAME PACKAGE_NAME PATH_SEPARATOR SHELL' ac_subst_files='' ac_user_opts=' enable_option_checking enable_silent_rules enable_dependency_tracking enable_largefile enable_threads enable_shared enable_static with_pic enable_fast_install with_aix_soname with_gnu_ld with_sysroot enable_libtool_lock enable_rpath with_libpth_prefix with_included_regex enable_gnulibcheck enable_arithmetic enable_buildprog enable_convertt enable_convolve enable_cosmiccal enable_crop enable_fits enable_match enable_mkcatalog enable_mknoise enable_mkprof 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Code from module connect: # Code from module connect-tests: # Code from module ctype: # Code from module ctype-tests: # Code from module dirname-lgpl: # Code from module dosname: # Code from module double-slash-root: # Code from module dup2: # Code from module dup2-tests: # Code from module environ: # Code from module environ-tests: # Code from module errno: # Code from module errno-tests: # Code from module error: # Code from module extensions: # Code from module extern-inline: # Code from module fcntl: # Code from module fcntl-h: # Code from module fcntl-h-tests: # Code from module fcntl-tests: # Code from module fd-hook: # Code from module fdl: # Code from module fdopen: # Code from module fdopen-tests: # Code from module fgetc-tests: # Code from module filename: # Code from module flexmember: # Code from module float: # Code from module float-tests: # Code from module fpieee: # Code from module fpucw: # Code from module fputc-tests: # Code from module fread-tests: # Code from module fstat: # Code from module fstat-tests: # Code from module ftruncate: # Code from module ftruncate-tests: # Code from module func: # Code from module func-tests: # Code from module fwrite-tests: # Code from module gendocs: # Code from module getcwd-lgpl: # Code from module getcwd-lgpl-tests: # Code from module getdelim: # Code from module getdelim-tests: # Code from module getdtablesize: # Code from module getdtablesize-tests: # Code from module getline: # Code from module getline-tests: # Code from module getopt-gnu: # Code from module getopt-gnu-tests: # Code from module getopt-posix: # Code from module getopt-posix-tests: # Code from module getpagesize: # Code from module getprogname: # Code from module getprogname-tests: # Code from module gettext-h: # Code from module gettimeofday: # Code from module gettimeofday-tests: # Code from module git-version-gen: # Code from module hard-locale: # Code from module havelib: # Code from module host-cpu-c-abi: # Code from module ignore-value: # Code from module ignore-value-tests: # Code from module include_next: # Code from module inet_pton: # Code from module inet_pton-tests: # Code from module intprops: # Code from module intprops-tests: # Code from module inttypes: # Code from module inttypes-incomplete: # Code from module inttypes-tests: # Code from module ioctl: # Code from module ioctl-tests: # Code from module isblank: # Code from module isblank-tests: # Code from module isnand-nolibm: # Code from module isnand-nolibm-tests: # Code from module isnanf-nolibm: # Code from module isnanf-nolibm-tests: # Code from module isnanl-nolibm: # Code from module isnanl-nolibm-tests: # Code from module iswblank: # Code from module iswblank-tests: # Code from module langinfo: # Code from module langinfo-tests: # Code from module largefile: # Code from module limits-h: # Code from module limits-h-tests: # Code from module listen: # Code from module listen-tests: # Code from module localcharset: # Code from module locale: # Code from module locale-tests: # Code from module localeconv: # Code from module localeconv-tests: # Code from module localename: # Code from module localename-tests: # Code from module localtime-buffer: # Code from module lock: # Code from module lock-tests: # Code from module lstat: # Code from module lstat-tests: # Code from module malloc-gnu: # Code from module malloc-gnu-tests: # Code from module malloc-posix: # Code from module malloca: # Code from module malloca-tests: # Code from module math: # Code from module math-tests: # Code from module mbchar: # Code from module mbrtowc: # Code from module mbrtowc-tests: # Code from module mbschr: # Code from module mbschr-tests: # Code from module mbsinit: # Code from module mbsinit-tests: # Code from module mbspbrk: # Code from module mbspbrk-tests: # Code from module mbsspn: # Code from module mbsspn-tests: # Code from module mbstok_r: # Code from module mbtowc: # Code from module mbuiter: # Code from module memchr: # Code from module memchr-tests: # Code from module mempcpy: # Code from module minmax: # Code from module msvc-inval: # Code from module msvc-nothrow: # Code from module multiarch: # Code from module nanosleep: # Code from module nanosleep-tests: # Code from module netinet_in: # Code from module netinet_in-tests: # Code from module nl_langinfo: # Code from module nl_langinfo-tests: # Code from module nocrash: # Code from module nproc: # Code from module open: # Code from module open-tests: # Code from module pathmax: # Code from module pathmax-tests: # Code from module perror: # Code from module perror-tests: # Code from module pipe-posix: # Code from module pipe-posix-tests: # Code from module pthread_sigmask: # Code from module pthread_sigmask-tests: # Code from module putenv: # Code from module raise: # Code from module raise-tests: # Code from module rawmemchr: # Code from module rawmemchr-tests: # Code from module regex: # Code from module regex-tests: # Code from module same-inode: # Code from module select: # Code from module select-tests: # Code from module setenv: # Code from module setenv-tests: # Code from module setlocale: # Code from module setlocale-tests: # Code from module setsockopt: # Code from module setsockopt-tests: # Code from module sigaction: # Code from module sigaction-tests: # Code from module signal-h: # Code from module signal-h-tests: # Code from module signbit: # Code from module signbit-tests: # Code from module sigprocmask: # Code from module sigprocmask-tests: # Code from module size_max: # Code from module sleep: # Code from module sleep-tests: # Code from module snippet/_Noreturn: # Code from module snippet/arg-nonnull: # Code from module snippet/c++defs: # Code from module snippet/warn-on-use: # Code from module socket: # Code from module socketlib: # Code from module sockets: # Code from module sockets-tests: # Code from module socklen: # Code from module ssize_t: # Code from module stat: # Code from module stat-tests: # Code from module stat-time: # Code from module stat-time-tests: # Code from module stdalign: # Code from module stdalign-tests: # Code from module stdbool: # Code from module stdbool-tests: # Code from module stddef: # Code from module stddef-tests: # Code from module stdint: # Code from module stdint-tests: # Code from module stdio: # Code from module stdio-tests: # Code from module stdlib: # Code from module stdlib-tests: # Code from module strcase: # Code from module strchrnul: # Code from module strchrnul-tests: # Code from module streq: # Code from module strerror: # Code from module strerror-override: # Code from module strerror-tests: # Code from module strerror_r-posix: # Code from module strerror_r-posix-tests: # Code from module string: # Code from module string-tests: # Code from module strings: # Code from module strings-tests: # Code from module strndup: # Code from module strnlen: # Code from module strnlen-tests: # Code from module strnlen1: # Code from module strtod: # Code from module strtod-tests: # Code from module strtok_r: # Code from module symlink: # Code from module symlink-tests: # Code from module sys_ioctl: # 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" >&6; } if ${lt_cv_to_tool_file_cmd+:} false; then : $as_echo_n "(cached) " >&6 else #assume ordinary cross tools, or native build. lt_cv_to_tool_file_cmd=func_convert_file_noop case $host in *-*-mingw* ) case $build in *-*-mingw* ) # actually msys lt_cv_to_tool_file_cmd=func_convert_file_msys_to_w32 ;; esac ;; esac fi to_tool_file_cmd=$lt_cv_to_tool_file_cmd { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_to_tool_file_cmd" >&5 $as_echo "$lt_cv_to_tool_file_cmd" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $LD option to reload object files" >&5 $as_echo_n "checking for $LD option to reload object files... " >&6; } if ${lt_cv_ld_reload_flag+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ld_reload_flag='-r' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ld_reload_flag" >&5 $as_echo "$lt_cv_ld_reload_flag" >&6; } reload_flag=$lt_cv_ld_reload_flag case $reload_flag in "" | " "*) ;; *) reload_flag=" $reload_flag" ;; esac reload_cmds='$LD$reload_flag -o $output$reload_objs' case $host_os in cygwin* | mingw* | pw32* | cegcc*) if test yes != "$GCC"; then reload_cmds=false fi ;; darwin*) if test yes = "$GCC"; then reload_cmds='$LTCC $LTCFLAGS -nostdlib $wl-r -o $output$reload_objs' else reload_cmds='$LD$reload_flag -o $output$reload_objs' fi ;; esac if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}objdump", so it can be a program name with args. set dummy ${ac_tool_prefix}objdump; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_OBJDUMP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$OBJDUMP"; then ac_cv_prog_OBJDUMP="$OBJDUMP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_OBJDUMP="${ac_tool_prefix}objdump" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi OBJDUMP=$ac_cv_prog_OBJDUMP if test -n "$OBJDUMP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $OBJDUMP" >&5 $as_echo "$OBJDUMP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_OBJDUMP"; then ac_ct_OBJDUMP=$OBJDUMP # Extract the first word of "objdump", so it can be a program name with args. set dummy objdump; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_OBJDUMP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_OBJDUMP"; then ac_cv_prog_ac_ct_OBJDUMP="$ac_ct_OBJDUMP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_OBJDUMP="objdump" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_OBJDUMP=$ac_cv_prog_ac_ct_OBJDUMP if test -n "$ac_ct_OBJDUMP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_OBJDUMP" >&5 $as_echo "$ac_ct_OBJDUMP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_OBJDUMP" = x; then OBJDUMP="false" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac OBJDUMP=$ac_ct_OBJDUMP fi else OBJDUMP="$ac_cv_prog_OBJDUMP" fi test -z "$OBJDUMP" && OBJDUMP=objdump { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to recognize dependent libraries" >&5 $as_echo_n "checking how to recognize dependent libraries... " >&6; } if ${lt_cv_deplibs_check_method+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_file_magic_cmd='$MAGIC_CMD' lt_cv_file_magic_test_file= lt_cv_deplibs_check_method='unknown' # Need to set the preceding variable on all platforms that support # interlibrary dependencies. # 'none' -- dependencies not supported. # 'unknown' -- same as none, but documents that we really don't know. # 'pass_all' -- all dependencies passed with no checks. # 'test_compile' -- check by making test program. # 'file_magic [[regex]]' -- check by looking for files in library path # that responds to the $file_magic_cmd with a given extended regex. # If you have 'file' or equivalent on your system and you're not sure # whether 'pass_all' will *always* work, you probably want this one. case $host_os in aix[4-9]*) lt_cv_deplibs_check_method=pass_all ;; beos*) lt_cv_deplibs_check_method=pass_all ;; bsdi[45]*) lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [ML]SB (shared object|dynamic lib)' lt_cv_file_magic_cmd='/usr/bin/file -L' lt_cv_file_magic_test_file=/shlib/libc.so ;; cygwin*) # func_win32_libid is a shell function defined in ltmain.sh lt_cv_deplibs_check_method='file_magic ^x86 archive import|^x86 DLL' lt_cv_file_magic_cmd='func_win32_libid' ;; mingw* | pw32*) # Base MSYS/MinGW do not provide the 'file' command needed by # func_win32_libid shell function, so use a weaker test based on 'objdump', # unless we find 'file', for example because we are cross-compiling. if ( file / ) >/dev/null 2>&1; then lt_cv_deplibs_check_method='file_magic ^x86 archive import|^x86 DLL' lt_cv_file_magic_cmd='func_win32_libid' else # Keep this pattern in sync with the one in func_win32_libid. lt_cv_deplibs_check_method='file_magic file format (pei*-i386(.*architecture: i386)?|pe-arm-wince|pe-x86-64)' lt_cv_file_magic_cmd='$OBJDUMP -f' fi ;; cegcc*) # use the weaker test based on 'objdump'. See mingw*. lt_cv_deplibs_check_method='file_magic file format pe-arm-.*little(.*architecture: arm)?' lt_cv_file_magic_cmd='$OBJDUMP -f' ;; darwin* | rhapsody*) lt_cv_deplibs_check_method=pass_all ;; freebsd* | dragonfly*) if echo __ELF__ | $CC -E - | $GREP __ELF__ > /dev/null; then case $host_cpu in i*86 ) # Not sure whether the presence of OpenBSD here was a mistake. # Let's accept both of them until this is cleared up. lt_cv_deplibs_check_method='file_magic (FreeBSD|OpenBSD|DragonFly)/i[3-9]86 (compact )?demand paged shared library' lt_cv_file_magic_cmd=/usr/bin/file lt_cv_file_magic_test_file=`echo /usr/lib/libc.so.*` ;; esac else lt_cv_deplibs_check_method=pass_all fi ;; haiku*) lt_cv_deplibs_check_method=pass_all ;; hpux10.20* | hpux11*) lt_cv_file_magic_cmd=/usr/bin/file case $host_cpu in ia64*) lt_cv_deplibs_check_method='file_magic (s[0-9][0-9][0-9]|ELF-[0-9][0-9]) shared object file - IA64' lt_cv_file_magic_test_file=/usr/lib/hpux32/libc.so ;; hppa*64*) lt_cv_deplibs_check_method='file_magic (s[0-9][0-9][0-9]|ELF[ -][0-9][0-9])(-bit)?( [LM]SB)? shared object( file)?[, -]* PA-RISC [0-9]\.[0-9]' lt_cv_file_magic_test_file=/usr/lib/pa20_64/libc.sl ;; *) lt_cv_deplibs_check_method='file_magic (s[0-9][0-9][0-9]|PA-RISC[0-9]\.[0-9]) shared library' lt_cv_file_magic_test_file=/usr/lib/libc.sl ;; esac ;; interix[3-9]*) # PIC code is broken on Interix 3.x, that's why |\.a not |_pic\.a here lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so|\.a)$' ;; irix5* | irix6* | nonstopux*) case $LD in *-32|*"-32 ") libmagic=32-bit;; *-n32|*"-n32 ") libmagic=N32;; *-64|*"-64 ") libmagic=64-bit;; *) libmagic=never-match;; esac lt_cv_deplibs_check_method=pass_all ;; # This must be glibc/ELF. linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) lt_cv_deplibs_check_method=pass_all ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ > /dev/null; then lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so\.[0-9]+\.[0-9]+|_pic\.a)$' else lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so|_pic\.a)$' fi ;; newos6*) lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [ML]SB (executable|dynamic lib)' lt_cv_file_magic_cmd=/usr/bin/file lt_cv_file_magic_test_file=/usr/lib/libnls.so ;; *nto* | *qnx*) lt_cv_deplibs_check_method=pass_all ;; openbsd* | bitrig*) if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so\.[0-9]+\.[0-9]+|\.so|_pic\.a)$' else lt_cv_deplibs_check_method='match_pattern /lib[^/]+(\.so\.[0-9]+\.[0-9]+|_pic\.a)$' fi ;; osf3* | osf4* | osf5*) lt_cv_deplibs_check_method=pass_all ;; rdos*) lt_cv_deplibs_check_method=pass_all ;; solaris*) lt_cv_deplibs_check_method=pass_all ;; sysv5* | sco3.2v5* | sco5v6* | unixware* | OpenUNIX* | sysv4*uw2*) lt_cv_deplibs_check_method=pass_all ;; sysv4 | sysv4.3*) case $host_vendor in motorola) lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [ML]SB (shared object|dynamic lib) M[0-9][0-9]* Version [0-9]' lt_cv_file_magic_test_file=`echo /usr/lib/libc.so*` ;; ncr) lt_cv_deplibs_check_method=pass_all ;; sequent) lt_cv_file_magic_cmd='/bin/file' lt_cv_deplibs_check_method='file_magic ELF [0-9][0-9]*-bit [LM]SB (shared object|dynamic lib )' ;; sni) lt_cv_file_magic_cmd='/bin/file' lt_cv_deplibs_check_method="file_magic ELF [0-9][0-9]*-bit [LM]SB dynamic lib" lt_cv_file_magic_test_file=/lib/libc.so ;; siemens) lt_cv_deplibs_check_method=pass_all ;; pc) lt_cv_deplibs_check_method=pass_all ;; esac ;; tpf*) lt_cv_deplibs_check_method=pass_all ;; os2*) lt_cv_deplibs_check_method=pass_all ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_deplibs_check_method" >&5 $as_echo "$lt_cv_deplibs_check_method" >&6; } file_magic_glob= want_nocaseglob=no if test "$build" = "$host"; then case $host_os in mingw* | pw32*) if ( shopt | grep nocaseglob ) >/dev/null 2>&1; then want_nocaseglob=yes else file_magic_glob=`echo aAbBcCdDeEfFgGhHiIjJkKlLmMnNoOpPqQrRsStTuUvVwWxXyYzZ | $SED -e "s/\(..\)/s\/[\1]\/[\1]\/g;/g"` fi ;; esac fi file_magic_cmd=$lt_cv_file_magic_cmd deplibs_check_method=$lt_cv_deplibs_check_method test -z "$deplibs_check_method" && deplibs_check_method=unknown if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}dlltool", so it can be a program name with args. set dummy ${ac_tool_prefix}dlltool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_DLLTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$DLLTOOL"; then ac_cv_prog_DLLTOOL="$DLLTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_DLLTOOL="${ac_tool_prefix}dlltool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi DLLTOOL=$ac_cv_prog_DLLTOOL if test -n "$DLLTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $DLLTOOL" >&5 $as_echo "$DLLTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_DLLTOOL"; then ac_ct_DLLTOOL=$DLLTOOL # Extract the first word of "dlltool", so it can be a program name with args. set dummy dlltool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_DLLTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_DLLTOOL"; then ac_cv_prog_ac_ct_DLLTOOL="$ac_ct_DLLTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_DLLTOOL="dlltool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_DLLTOOL=$ac_cv_prog_ac_ct_DLLTOOL if test -n "$ac_ct_DLLTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_DLLTOOL" >&5 $as_echo "$ac_ct_DLLTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_DLLTOOL" = x; then DLLTOOL="false" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac DLLTOOL=$ac_ct_DLLTOOL fi else DLLTOOL="$ac_cv_prog_DLLTOOL" fi test -z "$DLLTOOL" && DLLTOOL=dlltool { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to associate runtime and link libraries" >&5 $as_echo_n "checking how to associate runtime and link libraries... " >&6; } if ${lt_cv_sharedlib_from_linklib_cmd+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_sharedlib_from_linklib_cmd='unknown' case $host_os in cygwin* | mingw* | pw32* | cegcc*) # two different shell functions defined in ltmain.sh; # decide which one to use based on capabilities of $DLLTOOL case `$DLLTOOL --help 2>&1` in *--identify-strict*) lt_cv_sharedlib_from_linklib_cmd=func_cygming_dll_for_implib ;; *) lt_cv_sharedlib_from_linklib_cmd=func_cygming_dll_for_implib_fallback ;; esac ;; *) # fallback: assume linklib IS sharedlib lt_cv_sharedlib_from_linklib_cmd=$ECHO ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_sharedlib_from_linklib_cmd" >&5 $as_echo "$lt_cv_sharedlib_from_linklib_cmd" >&6; } sharedlib_from_linklib_cmd=$lt_cv_sharedlib_from_linklib_cmd test -z "$sharedlib_from_linklib_cmd" && sharedlib_from_linklib_cmd=$ECHO if test -n "$ac_tool_prefix"; then for ac_prog in ar do # Extract the first word of "$ac_tool_prefix$ac_prog", so it can be a program name with args. set dummy $ac_tool_prefix$ac_prog; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_AR+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$AR"; then ac_cv_prog_AR="$AR" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_AR="$ac_tool_prefix$ac_prog" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi AR=$ac_cv_prog_AR if test -n "$AR"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $AR" >&5 $as_echo "$AR" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi test -n "$AR" && break done fi if test -z "$AR"; then ac_ct_AR=$AR for ac_prog in ar do # Extract the first word of "$ac_prog", so it can be a program name with args. set dummy $ac_prog; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_AR+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_AR"; then ac_cv_prog_ac_ct_AR="$ac_ct_AR" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_AR="$ac_prog" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_AR=$ac_cv_prog_ac_ct_AR if test -n "$ac_ct_AR"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_AR" >&5 $as_echo "$ac_ct_AR" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi test -n "$ac_ct_AR" && break done if test "x$ac_ct_AR" = x; then AR="false" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac AR=$ac_ct_AR fi fi : ${AR=ar} # Use ARFLAGS variable as AR's operation code to sync the variable naming with # Automake. If both AR_FLAGS and ARFLAGS are specified, AR_FLAGS should have # higher priority because thats what people were doing historically (setting # ARFLAGS for automake and AR_FLAGS for libtool). FIXME: Make the AR_FLAGS # variable obsoleted/removed. test ${AR_FLAGS+y} || AR_FLAGS=${ARFLAGS-cr} lt_ar_flags=$AR_FLAGS # Make AR_FLAGS overridable by 'make ARFLAGS='. Don't try to run-time override # by AR_FLAGS because that was never working and AR_FLAGS is about to die. { $as_echo "$as_me:${as_lineno-$LINENO}: checking for archiver @FILE support" >&5 $as_echo_n "checking for archiver @FILE support... " >&6; } if ${lt_cv_ar_at_file+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ar_at_file=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : echo conftest.$ac_objext > conftest.lst lt_ar_try='$AR $AR_FLAGS libconftest.a @conftest.lst >&5' { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$lt_ar_try\""; } >&5 (eval $lt_ar_try) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } if test 0 -eq "$ac_status"; then # Ensure the archiver fails upon bogus file names. rm -f conftest.$ac_objext libconftest.a { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$lt_ar_try\""; } >&5 (eval $lt_ar_try) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } if test 0 -ne "$ac_status"; then lt_cv_ar_at_file=@ fi fi rm -f conftest.* libconftest.a fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ar_at_file" >&5 $as_echo "$lt_cv_ar_at_file" >&6; } if test no = "$lt_cv_ar_at_file"; then archiver_list_spec= else archiver_list_spec=$lt_cv_ar_at_file fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}strip", so it can be a program name with args. set dummy ${ac_tool_prefix}strip; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_STRIP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$STRIP"; then ac_cv_prog_STRIP="$STRIP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_STRIP="${ac_tool_prefix}strip" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi STRIP=$ac_cv_prog_STRIP if test -n "$STRIP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $STRIP" >&5 $as_echo "$STRIP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_STRIP"; then ac_ct_STRIP=$STRIP # Extract the first word of "strip", so it can be a program name with args. set dummy strip; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_STRIP+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_STRIP"; then ac_cv_prog_ac_ct_STRIP="$ac_ct_STRIP" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_STRIP="strip" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_STRIP=$ac_cv_prog_ac_ct_STRIP if test -n "$ac_ct_STRIP"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_STRIP" >&5 $as_echo "$ac_ct_STRIP" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_STRIP" = x; then STRIP=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac STRIP=$ac_ct_STRIP fi else STRIP="$ac_cv_prog_STRIP" fi test -z "$STRIP" && STRIP=: if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}ranlib", so it can be a program name with args. set dummy ${ac_tool_prefix}ranlib; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_RANLIB+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$RANLIB"; then ac_cv_prog_RANLIB="$RANLIB" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_RANLIB="${ac_tool_prefix}ranlib" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi RANLIB=$ac_cv_prog_RANLIB if test -n "$RANLIB"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $RANLIB" >&5 $as_echo "$RANLIB" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_RANLIB"; then ac_ct_RANLIB=$RANLIB # Extract the first word of "ranlib", so it can be a program name with args. set dummy ranlib; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_RANLIB+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_RANLIB"; then ac_cv_prog_ac_ct_RANLIB="$ac_ct_RANLIB" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_RANLIB="ranlib" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_RANLIB=$ac_cv_prog_ac_ct_RANLIB if test -n "$ac_ct_RANLIB"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_RANLIB" >&5 $as_echo "$ac_ct_RANLIB" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_RANLIB" = x; then RANLIB=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac RANLIB=$ac_ct_RANLIB fi else RANLIB="$ac_cv_prog_RANLIB" fi test -z "$RANLIB" && RANLIB=: # Determine commands to create old-style static archives. old_archive_cmds='$AR $AR_FLAGS $oldlib$oldobjs' old_postinstall_cmds='chmod 644 $oldlib' old_postuninstall_cmds= if test -n "$RANLIB"; then case $host_os in bitrig* | openbsd*) old_postinstall_cmds="$old_postinstall_cmds~\$RANLIB -t \$tool_oldlib" ;; *) old_postinstall_cmds="$old_postinstall_cmds~\$RANLIB \$tool_oldlib" ;; esac old_archive_cmds="$old_archive_cmds~\$RANLIB \$tool_oldlib" fi case $host_os in darwin*) lock_old_archive_extraction=yes ;; *) lock_old_archive_extraction=no ;; esac # If no C compiler was specified, use CC. LTCC=${LTCC-"$CC"} # If no C compiler flags were specified, use CFLAGS. LTCFLAGS=${LTCFLAGS-"$CFLAGS"} # Allow CC to be a program name with arguments. compiler=$CC # Check for command to grab the raw symbol name followed by C symbol from nm. { $as_echo "$as_me:${as_lineno-$LINENO}: checking command to parse $NM output from $compiler object" >&5 $as_echo_n "checking command to parse $NM output from $compiler object... " >&6; } if ${lt_cv_sys_global_symbol_pipe+:} false; then : $as_echo_n "(cached) " >&6 else # These are sane defaults that work on at least a few old systems. # [They come from Ultrix. What could be older than Ultrix?!! ;)] # Character class describing NM global symbol codes. symcode='[BCDEGRST]' # Regexp to match symbols that can be accessed directly from C. sympat='\([_A-Za-z][_A-Za-z0-9]*\)' # Define system-specific variables. case $host_os in aix*) symcode='[BCDT]' ;; cygwin* | mingw* | pw32* | cegcc*) symcode='[ABCDGISTW]' ;; hpux*) if test ia64 = "$host_cpu"; then symcode='[ABCDEGRST]' fi ;; irix* | nonstopux*) symcode='[BCDEGRST]' ;; osf*) symcode='[BCDEGQRST]' ;; solaris*) symcode='[BDRT]' ;; sco3.2v5*) symcode='[DT]' ;; sysv4.2uw2*) symcode='[DT]' ;; sysv5* | sco5v6* | unixware* | OpenUNIX*) symcode='[ABDT]' ;; sysv4) symcode='[DFNSTU]' ;; esac # If we're using GNU nm, then use its standard symbol codes. case `$NM -V 2>&1` in *GNU* | *'with BFD'*) symcode='[ABCDGIRSTW]' ;; esac if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Gets list of data symbols to import. lt_cv_sys_global_symbol_to_import="sed -n -e 's/^I .* \(.*\)$/\1/p'" # Adjust the below global symbol transforms to fixup imported variables. lt_cdecl_hook=" -e 's/^I .* \(.*\)$/extern __declspec(dllimport) char \1;/p'" lt_c_name_hook=" -e 's/^I .* \(.*\)$/ {\"\1\", (void *) 0},/p'" lt_c_name_lib_hook="\ -e 's/^I .* \(lib.*\)$/ {\"\1\", (void *) 0},/p'\ -e 's/^I .* \(.*\)$/ {\"lib\1\", (void *) 0},/p'" else # Disable hooks by default. lt_cv_sys_global_symbol_to_import= lt_cdecl_hook= lt_c_name_hook= lt_c_name_lib_hook= fi # Transform an extracted symbol line into a proper C declaration. # Some systems (esp. on ia64) link data and code symbols differently, # so use this general approach. lt_cv_sys_global_symbol_to_cdecl="sed -n"\ $lt_cdecl_hook\ " -e 's/^T .* \(.*\)$/extern int \1();/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/extern char \1;/p'" # Transform an extracted symbol line into symbol name and symbol address lt_cv_sys_global_symbol_to_c_name_address="sed -n"\ $lt_c_name_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/p'" # Transform an extracted symbol line into symbol name with lib prefix and # symbol address. lt_cv_sys_global_symbol_to_c_name_address_lib_prefix="sed -n"\ $lt_c_name_lib_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(lib.*\)$/ {\"\1\", (void *) \&\1},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"lib\1\", (void *) \&\1},/p'" # Handle CRLF in mingw tool chain opt_cr= case $build_os in mingw*) opt_cr=`$ECHO 'x\{0,1\}' | tr x '\015'` # option cr in regexp ;; esac # Try without a prefix underscore, then with it. for ac_symprfx in "" "_"; do # Transform symcode, sympat, and symprfx into a raw symbol and a C symbol. symxfrm="\\1 $ac_symprfx\\2 \\2" # Write the raw and C identifiers. if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Fake it for dumpbin and say T for any non-static function, # D for any global variable and I for any imported variable. # Also find C++ and __fastcall symbols from MSVC++, # which start with @ or ?. lt_cv_sys_global_symbol_pipe="$AWK '"\ " {last_section=section; section=\$ 3};"\ " /^COFF SYMBOL TABLE/{for(i in hide) delete hide[i]};"\ " /Section length .*#relocs.*(pick any)/{hide[last_section]=1};"\ " /^ *Symbol name *: /{split(\$ 0,sn,\":\"); si=substr(sn[2],2)};"\ " /^ *Type *: code/{print \"T\",si,substr(si,length(prfx))};"\ " /^ *Type *: data/{print \"I\",si,substr(si,length(prfx))};"\ " \$ 0!~/External *\|/{next};"\ " / 0+ UNDEF /{next}; / UNDEF \([^|]\)*()/{next};"\ " {if(hide[section]) next};"\ " {f=\"D\"}; \$ 0~/\(\).*\|/{f=\"T\"};"\ " {split(\$ 0,a,/\||\r/); split(a[2],s)};"\ " s[1]~/^[@?]/{print f,s[1],s[1]; next};"\ " s[1]~prfx {split(s[1],t,\"@\"); print f,t[1],substr(t[1],length(prfx))}"\ " ' prfx=^$ac_symprfx" else lt_cv_sys_global_symbol_pipe="sed -n -e 's/^.*[ ]\($symcode$symcode*\)[ ][ ]*$ac_symprfx$sympat$opt_cr$/$symxfrm/p'" fi lt_cv_sys_global_symbol_pipe="$lt_cv_sys_global_symbol_pipe | sed '/ __gnu_lto/d'" # Check to see that the pipe works correctly. pipe_works=no rm -f conftest* cat > conftest.$ac_ext <<_LT_EOF #ifdef __cplusplus extern "C" { #endif char nm_test_var; void nm_test_func(void); void nm_test_func(void){} #ifdef __cplusplus } #endif int main(){nm_test_var='a';nm_test_func();return(0);} _LT_EOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then # Now try to grab the symbols. nlist=conftest.nm if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$NM conftest.$ac_objext \| "$lt_cv_sys_global_symbol_pipe" \> $nlist\""; } >&5 (eval $NM conftest.$ac_objext \| "$lt_cv_sys_global_symbol_pipe" \> $nlist) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s "$nlist"; then # Try sorting and uniquifying the output. if sort "$nlist" | uniq > "$nlist"T; then mv -f "$nlist"T "$nlist" else rm -f "$nlist"T fi # Make sure that we snagged all the symbols we need. if $GREP ' nm_test_var$' "$nlist" >/dev/null; then if $GREP ' nm_test_func$' "$nlist" >/dev/null; then cat <<_LT_EOF > conftest.$ac_ext /* Keep this code in sync between libtool.m4, ltmain, lt_system.h, and tests. */ #if defined _WIN32 || defined __CYGWIN__ || defined _WIN32_WCE /* DATA imports from DLLs on WIN32 can't be const, because runtime relocations are performed -- see ld's documentation on pseudo-relocs. */ # define LT_DLSYM_CONST #elif defined __osf__ /* This system does not cope well with relocations in const data. */ # define LT_DLSYM_CONST #else # define LT_DLSYM_CONST const #endif #ifdef __cplusplus extern "C" { #endif _LT_EOF # Now generate the symbol file. eval "$lt_cv_sys_global_symbol_to_cdecl"' < "$nlist" | $GREP -v main >> conftest.$ac_ext' cat <<_LT_EOF >> conftest.$ac_ext /* The mapping between symbol names and symbols. */ LT_DLSYM_CONST struct { const char *name; void *address; } lt__PROGRAM__LTX_preloaded_symbols[] = { { "@PROGRAM@", (void *) 0 }, _LT_EOF $SED "s/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/" < "$nlist" | $GREP -v main >> conftest.$ac_ext cat <<\_LT_EOF >> conftest.$ac_ext {0, (void *) 0} }; /* This works around a problem in FreeBSD linker */ #ifdef FREEBSD_WORKAROUND static const void *lt_preloaded_setup() { return lt__PROGRAM__LTX_preloaded_symbols; } #endif #ifdef __cplusplus } #endif _LT_EOF # Now try linking the two files. mv conftest.$ac_objext conftstm.$ac_objext lt_globsym_save_LIBS=$LIBS lt_globsym_save_CFLAGS=$CFLAGS LIBS=conftstm.$ac_objext CFLAGS="$CFLAGS$lt_prog_compiler_no_builtin_flag" if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then pipe_works=yes fi LIBS=$lt_globsym_save_LIBS CFLAGS=$lt_globsym_save_CFLAGS else echo "cannot find nm_test_func in $nlist" >&5 fi else echo "cannot find nm_test_var in $nlist" >&5 fi else echo "cannot run $lt_cv_sys_global_symbol_pipe" >&5 fi else echo "$progname: failed program was:" >&5 cat conftest.$ac_ext >&5 fi rm -rf conftest* conftst* # Do not use the global_symbol_pipe unless it works. if test yes = "$pipe_works"; then break else lt_cv_sys_global_symbol_pipe= fi done fi if test -z "$lt_cv_sys_global_symbol_pipe"; then lt_cv_sys_global_symbol_to_cdecl= fi if test -z "$lt_cv_sys_global_symbol_pipe$lt_cv_sys_global_symbol_to_cdecl"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: failed" >&5 $as_echo "failed" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: ok" >&5 $as_echo "ok" >&6; } fi # Response file support. if test "$lt_cv_nm_interface" = "MS dumpbin"; then nm_file_list_spec='@' elif $NM --help 2>/dev/null | grep '[@]FILE' >/dev/null; then nm_file_list_spec='@' fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for sysroot" >&5 $as_echo_n "checking for sysroot... " >&6; } # Check whether --with-sysroot was given. if test "${with_sysroot+set}" = set; then : withval=$with_sysroot; else with_sysroot=no fi lt_sysroot= case $with_sysroot in #( yes) if test yes = "$GCC"; then lt_sysroot=`$CC --print-sysroot 2>/dev/null` fi ;; #( /*) lt_sysroot=`echo "$with_sysroot" | sed -e "$sed_quote_subst"` ;; #( no|'') ;; #( *) { $as_echo "$as_me:${as_lineno-$LINENO}: result: $with_sysroot" >&5 $as_echo "$with_sysroot" >&6; } as_fn_error $? "The sysroot must be an absolute path." "$LINENO" 5 ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: result: ${lt_sysroot:-no}" >&5 $as_echo "${lt_sysroot:-no}" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a working dd" >&5 $as_echo_n "checking for a working dd... " >&6; } if ${ac_cv_path_lt_DD+:} false; then : $as_echo_n "(cached) " >&6 else printf 0123456789abcdef0123456789abcdef >conftest.i cat conftest.i conftest.i >conftest2.i : ${lt_DD:=$DD} if test -z "$lt_DD"; then ac_path_lt_DD_found=false # Loop through the user's path and test for each of PROGNAME-LIST as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_prog in dd; do for ac_exec_ext in '' $ac_executable_extensions; do ac_path_lt_DD="$as_dir/$ac_prog$ac_exec_ext" as_fn_executable_p "$ac_path_lt_DD" || continue if "$ac_path_lt_DD" bs=32 count=1 conftest.out 2>/dev/null; then cmp -s conftest.i conftest.out \ && ac_cv_path_lt_DD="$ac_path_lt_DD" ac_path_lt_DD_found=: fi $ac_path_lt_DD_found && break 3 done done done IFS=$as_save_IFS if test -z "$ac_cv_path_lt_DD"; then : fi else ac_cv_path_lt_DD=$lt_DD fi rm -f conftest.i conftest2.i conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_path_lt_DD" >&5 $as_echo "$ac_cv_path_lt_DD" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to truncate binary pipes" >&5 $as_echo_n "checking how to truncate binary pipes... " >&6; } if ${lt_cv_truncate_bin+:} false; then : $as_echo_n "(cached) " >&6 else printf 0123456789abcdef0123456789abcdef >conftest.i cat conftest.i conftest.i >conftest2.i lt_cv_truncate_bin= if "$ac_cv_path_lt_DD" bs=32 count=1 conftest.out 2>/dev/null; then cmp -s conftest.i conftest.out \ && lt_cv_truncate_bin="$ac_cv_path_lt_DD bs=4096 count=1" fi rm -f conftest.i conftest2.i conftest.out test -z "$lt_cv_truncate_bin" && lt_cv_truncate_bin="$SED -e 4q" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_truncate_bin" >&5 $as_echo "$lt_cv_truncate_bin" >&6; } # Calculate cc_basename. Skip known compiler wrappers and cross-prefix. func_cc_basename () { for cc_temp in $*""; do case $cc_temp in compile | *[\\/]compile | ccache | *[\\/]ccache ) ;; distcc | *[\\/]distcc | purify | *[\\/]purify ) ;; \-*) ;; *) break;; esac done func_cc_basename_result=`$ECHO "$cc_temp" | $SED "s%.*/%%; s%^$host_alias-%%"` } # Check whether --enable-libtool-lock was given. if test "${enable_libtool_lock+set}" = set; then : enableval=$enable_libtool_lock; fi test no = "$enable_libtool_lock" || enable_libtool_lock=yes # Some flags need to be propagated to the compiler or linker for good # libtool support. case $host in ia64-*-hpux*) # Find out what ABI is being produced by ac_compile, and set mode # options accordingly. echo 'int i;' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then case `/usr/bin/file conftest.$ac_objext` in *ELF-32*) HPUX_IA64_MODE=32 ;; *ELF-64*) HPUX_IA64_MODE=64 ;; esac fi rm -rf conftest* ;; *-*-irix6*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. echo '#line '$LINENO' "configure"' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then if test yes = "$lt_cv_prog_gnu_ld"; then case `/usr/bin/file conftest.$ac_objext` in *32-bit*) LD="${LD-ld} -melf32bsmip" ;; *N32*) LD="${LD-ld} -melf32bmipn32" ;; *64-bit*) LD="${LD-ld} -melf64bmip" ;; esac else case `/usr/bin/file conftest.$ac_objext` in *32-bit*) LD="${LD-ld} -32" ;; *N32*) LD="${LD-ld} -n32" ;; *64-bit*) LD="${LD-ld} -64" ;; esac fi fi rm -rf conftest* ;; mips64*-*linux*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. echo '#line '$LINENO' "configure"' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then emul=elf case `/usr/bin/file conftest.$ac_objext` in *32-bit*) emul="${emul}32" ;; *64-bit*) emul="${emul}64" ;; esac case `/usr/bin/file conftest.$ac_objext` in *MSB*) emul="${emul}btsmip" ;; *LSB*) emul="${emul}ltsmip" ;; esac case `/usr/bin/file conftest.$ac_objext` in *N32*) emul="${emul}n32" ;; esac LD="${LD-ld} -m $emul" fi rm -rf conftest* ;; x86_64-*kfreebsd*-gnu|x86_64-*linux*|powerpc*-*linux*| \ s390*-*linux*|s390*-*tpf*|sparc*-*linux*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. Note that the listed cases only cover the # situations where additional linker options are needed (such as when # doing 32-bit compilation for a host where ld defaults to 64-bit, or # vice versa); the common cases where no linker options are needed do # not appear in the list. echo 'int i;' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then case `/usr/bin/file conftest.o` in *32-bit*) case $host in x86_64-*kfreebsd*-gnu) LD="${LD-ld} -m elf_i386_fbsd" ;; x86_64-*linux*) case `/usr/bin/file conftest.o` in *x86-64*) LD="${LD-ld} -m elf32_x86_64" ;; *) LD="${LD-ld} -m elf_i386" ;; esac ;; powerpc64le-*linux*) LD="${LD-ld} -m elf32lppclinux" ;; powerpc64-*linux*) LD="${LD-ld} -m elf32ppclinux" ;; s390x-*linux*) LD="${LD-ld} -m elf_s390" ;; sparc64-*linux*) LD="${LD-ld} -m elf32_sparc" ;; esac ;; *64-bit*) case $host in x86_64-*kfreebsd*-gnu) LD="${LD-ld} -m elf_x86_64_fbsd" ;; x86_64-*linux*) LD="${LD-ld} -m elf_x86_64" ;; powerpcle-*linux*) LD="${LD-ld} -m elf64lppc" ;; powerpc-*linux*) LD="${LD-ld} -m elf64ppc" ;; s390*-*linux*|s390*-*tpf*) LD="${LD-ld} -m elf64_s390" ;; sparc*-*linux*) LD="${LD-ld} -m elf64_sparc" ;; esac ;; esac fi rm -rf conftest* ;; *-*-sco3.2v5*) # On SCO OpenServer 5, we need -belf to get full-featured binaries. SAVE_CFLAGS=$CFLAGS CFLAGS="$CFLAGS -belf" { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether the C compiler needs -belf" >&5 $as_echo_n "checking whether the C compiler needs -belf... " >&6; } if ${lt_cv_cc_needs_belf+:} false; then : $as_echo_n "(cached) " >&6 else ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_cv_cc_needs_belf=yes else lt_cv_cc_needs_belf=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_cc_needs_belf" >&5 $as_echo "$lt_cv_cc_needs_belf" >&6; } if test yes != "$lt_cv_cc_needs_belf"; then # this is probably gcc 2.8.0, egcs 1.0 or newer; no need for -belf CFLAGS=$SAVE_CFLAGS fi ;; *-*solaris*) # Find out what ABI is being produced by ac_compile, and set linker # options accordingly. echo 'int i;' > conftest.$ac_ext if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_compile\""; } >&5 (eval $ac_compile) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; then case `/usr/bin/file conftest.o` in *64-bit*) case $lt_cv_prog_gnu_ld in yes*) case $host in i?86-*-solaris*|x86_64-*-solaris*) LD="${LD-ld} -m elf_x86_64" ;; sparc*-*-solaris*) LD="${LD-ld} -m elf64_sparc" ;; esac # GNU ld 2.21 introduced _sol2 emulations. Use them if available. if ${LD-ld} -V | grep _sol2 >/dev/null 2>&1; then LD=${LD-ld}_sol2 fi ;; *) if ${LD-ld} -64 -r -o conftest2.o conftest.o >/dev/null 2>&1; then LD="${LD-ld} -64" fi ;; esac ;; esac fi rm -rf conftest* ;; esac need_locks=$enable_libtool_lock if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}mt", so it can be a program name with args. set dummy ${ac_tool_prefix}mt; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_MANIFEST_TOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$MANIFEST_TOOL"; then ac_cv_prog_MANIFEST_TOOL="$MANIFEST_TOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_MANIFEST_TOOL="${ac_tool_prefix}mt" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi MANIFEST_TOOL=$ac_cv_prog_MANIFEST_TOOL if test -n "$MANIFEST_TOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $MANIFEST_TOOL" >&5 $as_echo "$MANIFEST_TOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_MANIFEST_TOOL"; then ac_ct_MANIFEST_TOOL=$MANIFEST_TOOL # Extract the first word of "mt", so it can be a program name with args. set dummy mt; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_MANIFEST_TOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_MANIFEST_TOOL"; then ac_cv_prog_ac_ct_MANIFEST_TOOL="$ac_ct_MANIFEST_TOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_MANIFEST_TOOL="mt" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_MANIFEST_TOOL=$ac_cv_prog_ac_ct_MANIFEST_TOOL if test -n "$ac_ct_MANIFEST_TOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_MANIFEST_TOOL" >&5 $as_echo "$ac_ct_MANIFEST_TOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_MANIFEST_TOOL" = x; then MANIFEST_TOOL=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac MANIFEST_TOOL=$ac_ct_MANIFEST_TOOL fi else MANIFEST_TOOL="$ac_cv_prog_MANIFEST_TOOL" fi test -z "$MANIFEST_TOOL" && MANIFEST_TOOL=mt { $as_echo "$as_me:${as_lineno-$LINENO}: checking if $MANIFEST_TOOL is a manifest tool" >&5 $as_echo_n "checking if $MANIFEST_TOOL is a manifest tool... " >&6; } if ${lt_cv_path_mainfest_tool+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_path_mainfest_tool=no echo "$as_me:$LINENO: $MANIFEST_TOOL '-?'" >&5 $MANIFEST_TOOL '-?' 2>conftest.err > conftest.out cat conftest.err >&5 if $GREP 'Manifest Tool' conftest.out > /dev/null; then lt_cv_path_mainfest_tool=yes fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_path_mainfest_tool" >&5 $as_echo "$lt_cv_path_mainfest_tool" >&6; } if test yes != "$lt_cv_path_mainfest_tool"; then MANIFEST_TOOL=: fi case $host_os in rhapsody* | darwin*) if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}dsymutil", so it can be a program name with args. set dummy ${ac_tool_prefix}dsymutil; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_DSYMUTIL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$DSYMUTIL"; then ac_cv_prog_DSYMUTIL="$DSYMUTIL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_DSYMUTIL="${ac_tool_prefix}dsymutil" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi DSYMUTIL=$ac_cv_prog_DSYMUTIL if test -n "$DSYMUTIL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $DSYMUTIL" >&5 $as_echo "$DSYMUTIL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_DSYMUTIL"; then ac_ct_DSYMUTIL=$DSYMUTIL # Extract the first word of "dsymutil", so it can be a program name with args. set dummy dsymutil; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_DSYMUTIL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_DSYMUTIL"; then ac_cv_prog_ac_ct_DSYMUTIL="$ac_ct_DSYMUTIL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_DSYMUTIL="dsymutil" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_DSYMUTIL=$ac_cv_prog_ac_ct_DSYMUTIL if test -n "$ac_ct_DSYMUTIL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_DSYMUTIL" >&5 $as_echo "$ac_ct_DSYMUTIL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_DSYMUTIL" = x; then DSYMUTIL=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac DSYMUTIL=$ac_ct_DSYMUTIL fi else DSYMUTIL="$ac_cv_prog_DSYMUTIL" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}nmedit", so it can be a program name with args. set dummy ${ac_tool_prefix}nmedit; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_NMEDIT+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$NMEDIT"; then ac_cv_prog_NMEDIT="$NMEDIT" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_NMEDIT="${ac_tool_prefix}nmedit" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi NMEDIT=$ac_cv_prog_NMEDIT if test -n "$NMEDIT"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $NMEDIT" >&5 $as_echo "$NMEDIT" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_NMEDIT"; then ac_ct_NMEDIT=$NMEDIT # Extract the first word of "nmedit", so it can be a program name with args. set dummy nmedit; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_NMEDIT+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_NMEDIT"; then ac_cv_prog_ac_ct_NMEDIT="$ac_ct_NMEDIT" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_NMEDIT="nmedit" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_NMEDIT=$ac_cv_prog_ac_ct_NMEDIT if test -n "$ac_ct_NMEDIT"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_NMEDIT" >&5 $as_echo "$ac_ct_NMEDIT" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_NMEDIT" = x; then NMEDIT=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac NMEDIT=$ac_ct_NMEDIT fi else NMEDIT="$ac_cv_prog_NMEDIT" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}lipo", so it can be a program name with args. set dummy ${ac_tool_prefix}lipo; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_LIPO+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$LIPO"; then ac_cv_prog_LIPO="$LIPO" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_LIPO="${ac_tool_prefix}lipo" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi LIPO=$ac_cv_prog_LIPO if test -n "$LIPO"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $LIPO" >&5 $as_echo "$LIPO" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_LIPO"; then ac_ct_LIPO=$LIPO # Extract the first word of "lipo", so it can be a program name with args. set dummy lipo; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_LIPO+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_LIPO"; then ac_cv_prog_ac_ct_LIPO="$ac_ct_LIPO" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_LIPO="lipo" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_LIPO=$ac_cv_prog_ac_ct_LIPO if test -n "$ac_ct_LIPO"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_LIPO" >&5 $as_echo "$ac_ct_LIPO" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_LIPO" = x; then LIPO=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac LIPO=$ac_ct_LIPO fi else LIPO="$ac_cv_prog_LIPO" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}otool", so it can be a program name with args. set dummy ${ac_tool_prefix}otool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_OTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$OTOOL"; then ac_cv_prog_OTOOL="$OTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_OTOOL="${ac_tool_prefix}otool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi OTOOL=$ac_cv_prog_OTOOL if test -n "$OTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $OTOOL" >&5 $as_echo "$OTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_OTOOL"; then ac_ct_OTOOL=$OTOOL # Extract the first word of "otool", so it can be a program name with args. set dummy otool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_OTOOL+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_OTOOL"; then ac_cv_prog_ac_ct_OTOOL="$ac_ct_OTOOL" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_OTOOL="otool" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_OTOOL=$ac_cv_prog_ac_ct_OTOOL if test -n "$ac_ct_OTOOL"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_OTOOL" >&5 $as_echo "$ac_ct_OTOOL" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_OTOOL" = x; then OTOOL=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac OTOOL=$ac_ct_OTOOL fi else OTOOL="$ac_cv_prog_OTOOL" fi if test -n "$ac_tool_prefix"; then # Extract the first word of "${ac_tool_prefix}otool64", so it can be a program name with args. set dummy ${ac_tool_prefix}otool64; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_OTOOL64+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$OTOOL64"; then ac_cv_prog_OTOOL64="$OTOOL64" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_OTOOL64="${ac_tool_prefix}otool64" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi OTOOL64=$ac_cv_prog_OTOOL64 if test -n "$OTOOL64"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $OTOOL64" >&5 $as_echo "$OTOOL64" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi fi if test -z "$ac_cv_prog_OTOOL64"; then ac_ct_OTOOL64=$OTOOL64 # Extract the first word of "otool64", so it can be a program name with args. set dummy otool64; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... " >&6; } if ${ac_cv_prog_ac_ct_OTOOL64+:} false; then : $as_echo_n "(cached) " >&6 else if test -n "$ac_ct_OTOOL64"; then ac_cv_prog_ac_ct_OTOOL64="$ac_ct_OTOOL64" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if as_fn_executable_p "$as_dir/$ac_word$ac_exec_ext"; then ac_cv_prog_ac_ct_OTOOL64="otool64" $as_echo "$as_me:${as_lineno-$LINENO}: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_OTOOL64=$ac_cv_prog_ac_ct_OTOOL64 if test -n "$ac_ct_OTOOL64"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_ct_OTOOL64" >&5 $as_echo "$ac_ct_OTOOL64" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test "x$ac_ct_OTOOL64" = x; then OTOOL64=":" else case $cross_compiling:$ac_tool_warned in yes:) { $as_echo "$as_me:${as_lineno-$LINENO}: WARNING: using cross tools not prefixed with host triplet" >&5 $as_echo "$as_me: WARNING: using cross tools not prefixed with host triplet" >&2;} ac_tool_warned=yes ;; esac OTOOL64=$ac_ct_OTOOL64 fi else OTOOL64="$ac_cv_prog_OTOOL64" fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for -single_module linker flag" >&5 $as_echo_n "checking for -single_module linker flag... " >&6; } if ${lt_cv_apple_cc_single_mod+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_apple_cc_single_mod=no if test -z "$LT_MULTI_MODULE"; then # By default we will add the -single_module flag. You can override # by either setting the environment variable LT_MULTI_MODULE # non-empty at configure time, or by adding -multi_module to the # link flags. rm -rf libconftest.dylib* echo "int foo(void){return 1;}" > conftest.c echo "$LTCC $LTCFLAGS $LDFLAGS -o libconftest.dylib \ -dynamiclib -Wl,-single_module conftest.c" >&5 $LTCC $LTCFLAGS $LDFLAGS -o libconftest.dylib \ -dynamiclib -Wl,-single_module conftest.c 2>conftest.err _lt_result=$? # If there is a non-empty error log, and "single_module" # appears in it, assume the flag caused a linker warning if test -s conftest.err && $GREP single_module conftest.err; then cat conftest.err >&5 # Otherwise, if the output was created with a 0 exit code from # the compiler, it worked. elif test -f libconftest.dylib && test 0 = "$_lt_result"; then lt_cv_apple_cc_single_mod=yes else cat conftest.err >&5 fi rm -rf libconftest.dylib* rm -f conftest.* fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_apple_cc_single_mod" >&5 $as_echo "$lt_cv_apple_cc_single_mod" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for -exported_symbols_list linker flag" >&5 $as_echo_n "checking for -exported_symbols_list linker flag... " >&6; } if ${lt_cv_ld_exported_symbols_list+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ld_exported_symbols_list=no save_LDFLAGS=$LDFLAGS echo "_main" > conftest.sym LDFLAGS="$LDFLAGS -Wl,-exported_symbols_list,conftest.sym" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_cv_ld_exported_symbols_list=yes else lt_cv_ld_exported_symbols_list=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LDFLAGS=$save_LDFLAGS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ld_exported_symbols_list" >&5 $as_echo "$lt_cv_ld_exported_symbols_list" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for -force_load linker flag" >&5 $as_echo_n "checking for -force_load linker flag... " >&6; } if ${lt_cv_ld_force_load+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_ld_force_load=no cat > conftest.c << _LT_EOF int forced_loaded() { return 2;} _LT_EOF echo "$LTCC $LTCFLAGS -c -o conftest.o conftest.c" >&5 $LTCC $LTCFLAGS -c -o conftest.o conftest.c 2>&5 echo "$AR $AR_FLAGS libconftest.a conftest.o" >&5 $AR $AR_FLAGS libconftest.a conftest.o 2>&5 echo "$RANLIB libconftest.a" >&5 $RANLIB libconftest.a 2>&5 cat > conftest.c << _LT_EOF int main() { return 0;} _LT_EOF echo "$LTCC $LTCFLAGS $LDFLAGS -o conftest conftest.c -Wl,-force_load,./libconftest.a" >&5 $LTCC $LTCFLAGS $LDFLAGS -o conftest conftest.c -Wl,-force_load,./libconftest.a 2>conftest.err _lt_result=$? if test -s conftest.err && $GREP force_load conftest.err; then cat conftest.err >&5 elif test -f conftest && test 0 = "$_lt_result" && $GREP forced_load conftest >/dev/null 2>&1; then lt_cv_ld_force_load=yes else cat conftest.err >&5 fi rm -f conftest.err libconftest.a conftest conftest.c rm -rf conftest.dSYM fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_ld_force_load" >&5 $as_echo "$lt_cv_ld_force_load" >&6; } case $host_os in rhapsody* | darwin1.[012]) _lt_dar_allow_undefined='$wl-undefined ${wl}suppress' ;; darwin1.*) _lt_dar_allow_undefined='$wl-flat_namespace $wl-undefined ${wl}suppress' ;; darwin*) # darwin 5.x on # if running on 10.5 or later, the deployment target defaults # to the OS version, if on x86, and 10.4, the deployment # target defaults to 10.4. Don't you love it? case ${MACOSX_DEPLOYMENT_TARGET-10.0},$host in 10.0,*86*-darwin8*|10.0,*-darwin[91]*) _lt_dar_allow_undefined='$wl-undefined ${wl}dynamic_lookup' ;; 10.[012][,.]*) _lt_dar_allow_undefined='$wl-flat_namespace $wl-undefined ${wl}suppress' ;; 10.*) _lt_dar_allow_undefined='$wl-undefined ${wl}dynamic_lookup' ;; esac ;; esac if test yes = "$lt_cv_apple_cc_single_mod"; then _lt_dar_single_mod='$single_module' fi if test yes = "$lt_cv_ld_exported_symbols_list"; then _lt_dar_export_syms=' $wl-exported_symbols_list,$output_objdir/$libname-symbols.expsym' else _lt_dar_export_syms='~$NMEDIT -s $output_objdir/$libname-symbols.expsym $lib' fi if test : != "$DSYMUTIL" && test no = "$lt_cv_ld_force_load"; then _lt_dsymutil='~$DSYMUTIL $lib || :' else _lt_dsymutil= fi ;; esac # func_munge_path_list VARIABLE PATH # ----------------------------------- # VARIABLE is name of variable containing _space_ separated list of # directories to be munged by the contents of PATH, which is string # having a format: # "DIR[:DIR]:" # string "DIR[ DIR]" will be prepended to VARIABLE # ":DIR[:DIR]" # string "DIR[ DIR]" will be appended to VARIABLE # "DIRP[:DIRP]::[DIRA:]DIRA" # string "DIRP[ DIRP]" will be prepended to VARIABLE and string # "DIRA[ DIRA]" will be appended to VARIABLE # "DIR[:DIR]" # VARIABLE will be replaced by "DIR[ DIR]" func_munge_path_list () { case x$2 in x) ;; *:) eval $1=\"`$ECHO $2 | $SED 's/:/ /g'` \$$1\" ;; x:*) eval $1=\"\$$1 `$ECHO $2 | $SED 's/:/ /g'`\" ;; *::*) eval $1=\"\$$1\ `$ECHO $2 | $SED -e 's/.*:://' -e 's/:/ /g'`\" eval $1=\"`$ECHO $2 | $SED -e 's/::.*//' -e 's/:/ /g'`\ \$$1\" ;; *) eval $1=\"`$ECHO $2 | $SED 's/:/ /g'`\" ;; esac } for ac_header in dlfcn.h do : ac_fn_c_check_header_compile "$LINENO" "dlfcn.h" "ac_cv_header_dlfcn_h" "$ac_includes_default " if test "x$ac_cv_header_dlfcn_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_DLFCN_H 1 _ACEOF fi done func_stripname_cnf () { case $2 in .*) func_stripname_result=`$ECHO "$3" | $SED "s%^$1%%; s%\\\\$2\$%%"`;; *) func_stripname_result=`$ECHO "$3" | $SED "s%^$1%%; s%$2\$%%"`;; esac } # func_stripname_cnf # Set options enable_dlopen=no enable_win32_dll=no # Check whether --enable-shared was given. if test "${enable_shared+set}" = set; then : enableval=$enable_shared; p=${PACKAGE-default} case $enableval in yes) enable_shared=yes ;; no) enable_shared=no ;; *) enable_shared=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_shared=yes fi done IFS=$lt_save_ifs ;; esac else enable_shared=yes fi # Check whether --enable-static was given. if test "${enable_static+set}" = set; then : enableval=$enable_static; p=${PACKAGE-default} case $enableval in yes) enable_static=yes ;; no) enable_static=no ;; *) enable_static=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_static=yes fi done IFS=$lt_save_ifs ;; esac else enable_static=yes fi # Check whether --with-pic was given. if test "${with_pic+set}" = set; then : withval=$with_pic; lt_p=${PACKAGE-default} case $withval in yes|no) pic_mode=$withval ;; *) pic_mode=default # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for lt_pkg in $withval; do IFS=$lt_save_ifs if test "X$lt_pkg" = "X$lt_p"; then pic_mode=yes fi done IFS=$lt_save_ifs ;; esac else pic_mode=default fi # Check whether --enable-fast-install was given. if test "${enable_fast_install+set}" = set; then : enableval=$enable_fast_install; p=${PACKAGE-default} case $enableval in yes) enable_fast_install=yes ;; no) enable_fast_install=no ;; *) enable_fast_install=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_fast_install=yes fi done IFS=$lt_save_ifs ;; esac else enable_fast_install=yes fi shared_archive_member_spec= case $host,$enable_shared in power*-*-aix[5-9]*,yes) { $as_echo "$as_me:${as_lineno-$LINENO}: checking which variant of shared library versioning to provide" >&5 $as_echo_n "checking which variant of shared library versioning to provide... " >&6; } # Check whether --with-aix-soname was given. if test "${with_aix_soname+set}" = set; then : withval=$with_aix_soname; case $withval in aix|svr4|both) ;; *) as_fn_error $? "Unknown argument to --with-aix-soname" "$LINENO" 5 ;; esac lt_cv_with_aix_soname=$with_aix_soname else if ${lt_cv_with_aix_soname+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_with_aix_soname=aix fi with_aix_soname=$lt_cv_with_aix_soname fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $with_aix_soname" >&5 $as_echo "$with_aix_soname" >&6; } if test aix != "$with_aix_soname"; then # For the AIX way of multilib, we name the shared archive member # based on the bitwidth used, traditionally 'shr.o' or 'shr_64.o', # and 'shr.imp' or 'shr_64.imp', respectively, for the Import File. # Even when GNU compilers ignore OBJECT_MODE but need '-maix64' flag, # the AIX toolchain works better with OBJECT_MODE set (default 32). if test 64 = "${OBJECT_MODE-32}"; then shared_archive_member_spec=shr_64 else shared_archive_member_spec=shr fi fi ;; *) with_aix_soname=aix ;; esac # This can be used to rebuild libtool when needed LIBTOOL_DEPS=$ltmain # Always use our own libtool. LIBTOOL='$(SHELL) $(top_builddir)/libtool' test -z "$LN_S" && LN_S="ln -s" if test -n "${ZSH_VERSION+set}"; then setopt NO_GLOB_SUBST fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for objdir" >&5 $as_echo_n "checking for objdir... " >&6; } if ${lt_cv_objdir+:} false; then : $as_echo_n "(cached) " >&6 else rm -f .libs 2>/dev/null mkdir .libs 2>/dev/null if test -d .libs; then lt_cv_objdir=.libs else # MS-DOS does not allow filenames that begin with a dot. lt_cv_objdir=_libs fi rmdir .libs 2>/dev/null fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_objdir" >&5 $as_echo "$lt_cv_objdir" >&6; } objdir=$lt_cv_objdir cat >>confdefs.h <<_ACEOF #define LT_OBJDIR "$lt_cv_objdir/" _ACEOF case $host_os in aix3*) # AIX sometimes has problems with the GCC collect2 program. 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This will affect the creation of libtool libraries that *** depend on shared libraries, but programs linked with such libtool *** libraries will work regardless of this problem. Nevertheless, you *** may want to report the problem to your system manager and/or to *** bug-libtool@gnu.org _LT_EOF fi ;; esac fi break fi done IFS=$lt_save_ifs MAGIC_CMD=$lt_save_MAGIC_CMD ;; esac fi MAGIC_CMD=$lt_cv_path_MAGIC_CMD if test -n "$MAGIC_CMD"; then { $as_echo "$as_me:${as_lineno-$LINENO}: result: $MAGIC_CMD" >&5 $as_echo "$MAGIC_CMD" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi if test -z "$lt_cv_path_MAGIC_CMD"; then if test -n "$ac_tool_prefix"; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for file" >&5 $as_echo_n "checking for file... 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We urge you to upgrade GNU *** binutils to release 2.16.91.0.3 or newer. Another option is to modify *** your PATH or compiler configuration so that the native linker is *** used, and then restart. _LT_EOF ;; *) # For security reasons, it is highly recommended that you always # use absolute paths for naming shared libraries, and exclude the # DT_RUNPATH tag from executables and libraries. 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If linking a library # or program results in "error TOC overflow" add -mminimal-toc to # CXXFLAGS/CFLAGS for g++/gcc. 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The following line is correct: shared_flag='-G' else if test yes = "$aix_use_runtimelinking"; then shared_flag='$wl-G' else shared_flag='$wl-bM:SRE' fi shared_flag_aix='$wl-bM:SRE' shared_flag_svr4='$wl-G' fi fi export_dynamic_flag_spec='$wl-bexpall' # It seems that -bexpall does not export symbols beginning with # underscore (_), so it is better to generate a list of symbols to export. always_export_symbols=yes if test aix,yes = "$with_aix_soname,$aix_use_runtimelinking"; then # Warning - without using the other runtime loading flags (-brtl), # -berok will link without error, but may produce a broken library. allow_undefined_flag='-berok' # Determine the default libpath from the value encoded in an # empty executable. if test set = "${lt_cv_aix_libpath+set}"; then aix_libpath=$lt_cv_aix_libpath else if ${lt_cv_aix_libpath_+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_aix_libpath_sed=' /Import File Strings/,/^$/ { /^0/ { s/^0 *\([^ ]*\) *$/\1/ p } }' lt_cv_aix_libpath_=`dump -H conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` # Check for a 64-bit object if we didn't find anything. if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=`dump -HX64 conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` fi fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=/usr/lib:/lib fi fi aix_libpath=$lt_cv_aix_libpath_ fi hardcode_libdir_flag_spec='$wl-blibpath:$libdir:'"$aix_libpath" archive_expsym_cmds='$CC -o $output_objdir/$soname $libobjs $deplibs $wl'$no_entry_flag' $compiler_flags `if test -n "$allow_undefined_flag"; then func_echo_all "$wl$allow_undefined_flag"; else :; fi` $wl'$exp_sym_flag:\$export_symbols' '$shared_flag else if test ia64 = "$host_cpu"; then hardcode_libdir_flag_spec='$wl-R $libdir:/usr/lib:/lib' allow_undefined_flag="-z nodefs" archive_expsym_cmds="\$CC $shared_flag"' -o $output_objdir/$soname $libobjs $deplibs '"\$wl$no_entry_flag"' $compiler_flags $wl$allow_undefined_flag '"\$wl$exp_sym_flag:\$export_symbols" else # Determine the default libpath from the value encoded in an # empty executable. if test set = "${lt_cv_aix_libpath+set}"; then aix_libpath=$lt_cv_aix_libpath else if ${lt_cv_aix_libpath_+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_aix_libpath_sed=' /Import File Strings/,/^$/ { /^0/ { s/^0 *\([^ ]*\) *$/\1/ p } }' lt_cv_aix_libpath_=`dump -H conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` # Check for a 64-bit object if we didn't find anything. if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=`dump -HX64 conftest$ac_exeext 2>/dev/null | $SED -n -e "$lt_aix_libpath_sed"` fi fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$lt_cv_aix_libpath_"; then lt_cv_aix_libpath_=/usr/lib:/lib fi fi aix_libpath=$lt_cv_aix_libpath_ fi hardcode_libdir_flag_spec='$wl-blibpath:$libdir:'"$aix_libpath" # Warning - without using the other run time loading flags, # -berok will link without error, but may produce a broken library. no_undefined_flag=' $wl-bernotok' allow_undefined_flag=' $wl-berok' if test yes = "$with_gnu_ld"; then # We only use this code for GNU lds that support --whole-archive. whole_archive_flag_spec='$wl--whole-archive$convenience $wl--no-whole-archive' else # Exported symbols can be pulled into shared objects from archives whole_archive_flag_spec='$convenience' fi archive_cmds_need_lc=yes archive_expsym_cmds='$RM -r $output_objdir/$realname.d~$MKDIR $output_objdir/$realname.d' # -brtl affects multiple linker settings, -berok does not and is overridden later compiler_flags_filtered='`func_echo_all "$compiler_flags " | $SED -e "s%-brtl\\([, ]\\)%-berok\\1%g"`' if test svr4 != "$with_aix_soname"; then # This is similar to how AIX traditionally builds its shared libraries. archive_expsym_cmds="$archive_expsym_cmds"'~$CC '$shared_flag_aix' -o $output_objdir/$realname.d/$soname $libobjs $deplibs $wl-bnoentry '$compiler_flags_filtered'$wl-bE:$export_symbols$allow_undefined_flag~$AR $AR_FLAGS $output_objdir/$libname$release.a $output_objdir/$realname.d/$soname' fi if test aix != "$with_aix_soname"; then archive_expsym_cmds="$archive_expsym_cmds"'~$CC '$shared_flag_svr4' -o $output_objdir/$realname.d/$shared_archive_member_spec.o $libobjs $deplibs $wl-bnoentry '$compiler_flags_filtered'$wl-bE:$export_symbols$allow_undefined_flag~$STRIP -e $output_objdir/$realname.d/$shared_archive_member_spec.o~( func_echo_all "#! $soname($shared_archive_member_spec.o)"; if test shr_64 = "$shared_archive_member_spec"; then func_echo_all "# 64"; else func_echo_all "# 32"; fi; cat $export_symbols ) > $output_objdir/$realname.d/$shared_archive_member_spec.imp~$AR $AR_FLAGS $output_objdir/$soname $output_objdir/$realname.d/$shared_archive_member_spec.o $output_objdir/$realname.d/$shared_archive_member_spec.imp' else # used by -dlpreopen to get the symbols archive_expsym_cmds="$archive_expsym_cmds"'~$MV $output_objdir/$realname.d/$soname $output_objdir' fi archive_expsym_cmds="$archive_expsym_cmds"'~$RM -r $output_objdir/$realname.d' fi fi ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' archive_expsym_cmds='' ;; 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then cp "$export_symbols" "$output_objdir/$soname.def"; echo "$tool_output_objdir$soname.def" > "$output_objdir/$soname.exp"; else $SED -e '\''s/^/-link -EXPORT:/'\'' < $export_symbols > $output_objdir/$soname.exp; fi~ $CC -o $tool_output_objdir$soname $libobjs $compiler_flags $deplibs "@$tool_output_objdir$soname.exp" -Wl,-DLL,-IMPLIB:"$tool_output_objdir$libname.dll.lib"~ linknames=' # The linker will not automatically build a static lib if we build a DLL. # _LT_TAGVAR(old_archive_from_new_cmds, )='true' enable_shared_with_static_runtimes=yes exclude_expsyms='_NULL_IMPORT_DESCRIPTOR|_IMPORT_DESCRIPTOR_.*' export_symbols_cmds='$NM $libobjs $convenience | $global_symbol_pipe | $SED -e '\''/^[BCDGRS][ ]/s/.*[ ]\([^ ]*\)/\1,DATA/'\'' | $SED -e '\''/^[AITW][ ]/s/.*[ ]//'\'' | sort | uniq > $export_symbols' # Don't use ranlib old_postinstall_cmds='chmod 644 $oldlib' postlink_cmds='lt_outputfile="@OUTPUT@"~ lt_tool_outputfile="@TOOL_OUTPUT@"~ case $lt_outputfile in *.exe|*.EXE) ;; *) lt_outputfile=$lt_outputfile.exe lt_tool_outputfile=$lt_tool_outputfile.exe ;; 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dgux*) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_libdir_flag_spec='-L$libdir' hardcode_shlibpath_var=no ;; # FreeBSD 2.2.[012] allows us to include c++rt0.o to get C++ constructor # support. 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" >&6; } if ${lt_cv_irix_exported_symbol+:} false; then : $as_echo_n "(cached) " >&6 else save_LDFLAGS=$LDFLAGS LDFLAGS="$LDFLAGS -shared $wl-exported_symbol ${wl}foo $wl-update_registry $wl/dev/null" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int foo (void) { return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : lt_cv_irix_exported_symbol=yes else lt_cv_irix_exported_symbol=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LDFLAGS=$save_LDFLAGS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $lt_cv_irix_exported_symbol" >&5 $as_echo "$lt_cv_irix_exported_symbol" >&6; } if test yes = "$lt_cv_irix_exported_symbol"; then archive_expsym_cmds='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname `test -n "$verstring" && func_echo_all "$wl-set_version $wl$verstring"` $wl-update_registry $wl$output_objdir/so_locations $wl-exports_file $wl$export_symbols -o $lib' fi else archive_cmds='$CC -shared $libobjs $deplibs $compiler_flags -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib' archive_expsym_cmds='$CC -shared $libobjs $deplibs $compiler_flags -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -exports_file $export_symbols -o $lib' fi archive_cmds_need_lc='no' hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' hardcode_libdir_separator=: inherit_rpath=yes link_all_deplibs=yes ;; linux*) case $cc_basename in tcc*) # Fabrice Bellard et al's Tiny C Compiler ld_shlibs=yes archive_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' ;; esac ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then archive_cmds='$LD -Bshareable -o $lib $libobjs $deplibs $linker_flags' # a.out else archive_cmds='$LD -shared -o $lib $libobjs $deplibs $linker_flags' # ELF fi hardcode_libdir_flag_spec='-R$libdir' hardcode_direct=yes hardcode_shlibpath_var=no ;; newsos6) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_direct=yes hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' hardcode_libdir_separator=: hardcode_shlibpath_var=no ;; *nto* | *qnx*) ;; openbsd* | bitrig*) if test -f /usr/libexec/ld.so; then hardcode_direct=yes hardcode_shlibpath_var=no hardcode_direct_absolute=yes if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then archive_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' archive_expsym_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags $wl-retain-symbols-file,$export_symbols' hardcode_libdir_flag_spec='$wl-rpath,$libdir' export_dynamic_flag_spec='$wl-E' else archive_cmds='$CC -shared $pic_flag -o $lib $libobjs $deplibs $compiler_flags' hardcode_libdir_flag_spec='$wl-rpath,$libdir' fi else ld_shlibs=no fi ;; os2*) hardcode_libdir_flag_spec='-L$libdir' hardcode_minus_L=yes allow_undefined_flag=unsupported shrext_cmds=.dll archive_cmds='$ECHO "LIBRARY ${soname%$shared_ext} INITINSTANCE TERMINSTANCE" > $output_objdir/$libname.def~ $ECHO "DESCRIPTION \"$libname\"" >> $output_objdir/$libname.def~ $ECHO "DATA MULTIPLE NONSHARED" >> $output_objdir/$libname.def~ $ECHO EXPORTS >> $output_objdir/$libname.def~ emxexp $libobjs | $SED /"_DLL_InitTerm"/d >> $output_objdir/$libname.def~ $CC -Zdll -Zcrtdll -o $output_objdir/$soname $libobjs $deplibs $compiler_flags $output_objdir/$libname.def~ emximp -o $lib $output_objdir/$libname.def' archive_expsym_cmds='$ECHO "LIBRARY ${soname%$shared_ext} INITINSTANCE TERMINSTANCE" > $output_objdir/$libname.def~ $ECHO "DESCRIPTION \"$libname\"" >> $output_objdir/$libname.def~ $ECHO "DATA MULTIPLE NONSHARED" >> $output_objdir/$libname.def~ $ECHO EXPORTS >> $output_objdir/$libname.def~ prefix_cmds="$SED"~ if test EXPORTS = "`$SED 1q $export_symbols`"; then prefix_cmds="$prefix_cmds -e 1d"; fi~ prefix_cmds="$prefix_cmds -e \"s/^\(.*\)$/_\1/g\""~ cat $export_symbols | $prefix_cmds >> $output_objdir/$libname.def~ $CC -Zdll -Zcrtdll -o $output_objdir/$soname $libobjs $deplibs $compiler_flags $output_objdir/$libname.def~ emximp -o $lib $output_objdir/$libname.def' old_archive_From_new_cmds='emximp -o $output_objdir/${libname}_dll.a $output_objdir/$libname.def' enable_shared_with_static_runtimes=yes file_list_spec='@' ;; osf3*) if test yes = "$GCC"; then allow_undefined_flag=' $wl-expect_unresolved $wl\*' archive_cmds='$CC -shared$allow_undefined_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname `test -n "$verstring" && func_echo_all "$wl-set_version $wl$verstring"` $wl-update_registry $wl$output_objdir/so_locations -o $lib' else allow_undefined_flag=' -expect_unresolved \*' archive_cmds='$CC -shared$allow_undefined_flag $libobjs $deplibs $compiler_flags -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib' fi archive_cmds_need_lc='no' hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' hardcode_libdir_separator=: ;; osf4* | osf5*) # as osf3* with the addition of -msym flag if test yes = "$GCC"; then allow_undefined_flag=' $wl-expect_unresolved $wl\*' archive_cmds='$CC -shared$allow_undefined_flag $pic_flag $libobjs $deplibs $compiler_flags $wl-msym $wl-soname $wl$soname `test -n "$verstring" && func_echo_all "$wl-set_version $wl$verstring"` $wl-update_registry $wl$output_objdir/so_locations -o $lib' hardcode_libdir_flag_spec='$wl-rpath $wl$libdir' else allow_undefined_flag=' -expect_unresolved \*' archive_cmds='$CC -shared$allow_undefined_flag $libobjs $deplibs $compiler_flags -msym -soname $soname `test -n "$verstring" && func_echo_all "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib' archive_expsym_cmds='for i in `cat $export_symbols`; do printf "%s %s\\n" -exported_symbol "\$i" >> $lib.exp; done; printf "%s\\n" "-hidden">> $lib.exp~ $CC -shared$allow_undefined_flag $wl-input $wl$lib.exp $compiler_flags $libobjs $deplibs -soname $soname `test -n "$verstring" && $ECHO "-set_version $verstring"` -update_registry $output_objdir/so_locations -o $lib~$RM $lib.exp' # Both c and cxx compiler support -rpath directly hardcode_libdir_flag_spec='-rpath $libdir' fi archive_cmds_need_lc='no' hardcode_libdir_separator=: ;; solaris*) no_undefined_flag=' -z defs' if test yes = "$GCC"; then wlarc='$wl' archive_cmds='$CC -shared $pic_flag $wl-z ${wl}text $wl-h $wl$soname -o $lib $libobjs $deplibs $compiler_flags' archive_expsym_cmds='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $CC -shared $pic_flag $wl-z ${wl}text $wl-M $wl$lib.exp $wl-h $wl$soname -o $lib $libobjs $deplibs $compiler_flags~$RM $lib.exp' else case `$CC -V 2>&1` in *"Compilers 5.0"*) wlarc='' archive_cmds='$LD -G$allow_undefined_flag -h $soname -o $lib $libobjs $deplibs $linker_flags' archive_expsym_cmds='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $LD -G$allow_undefined_flag -M $lib.exp -h $soname -o $lib $libobjs $deplibs $linker_flags~$RM $lib.exp' ;; *) wlarc='$wl' archive_cmds='$CC -G$allow_undefined_flag -h $soname -o $lib $libobjs $deplibs $compiler_flags' archive_expsym_cmds='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $CC -G$allow_undefined_flag -M $lib.exp -h $soname -o $lib $libobjs $deplibs $compiler_flags~$RM $lib.exp' ;; esac fi hardcode_libdir_flag_spec='-R$libdir' hardcode_shlibpath_var=no case $host_os in solaris2.[0-5] | solaris2.[0-5].*) ;; *) # The compiler driver will combine and reorder linker options, # but understands '-z linker_flag'. GCC discards it without '$wl', # but is careful enough not to reorder. # Supported since Solaris 2.6 (maybe 2.5.1?) if test yes = "$GCC"; then whole_archive_flag_spec='$wl-z ${wl}allextract$convenience $wl-z ${wl}defaultextract' else whole_archive_flag_spec='-z allextract$convenience -z defaultextract' fi ;; esac link_all_deplibs=yes ;; sunos4*) if test sequent = "$host_vendor"; then # Use $CC to link under sequent, because it throws in some extra .o # files that make .init and .fini sections work. archive_cmds='$CC -G $wl-h $soname -o $lib $libobjs $deplibs $compiler_flags' else archive_cmds='$LD -assert pure-text -Bstatic -o $lib $libobjs $deplibs $linker_flags' fi hardcode_libdir_flag_spec='-L$libdir' hardcode_direct=yes hardcode_minus_L=yes hardcode_shlibpath_var=no ;; sysv4) case $host_vendor in sni) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_direct=yes # is this really true??? ;; siemens) ## LD is ld it makes a PLAMLIB ## CC just makes a GrossModule. archive_cmds='$LD -G -o $lib $libobjs $deplibs $linker_flags' reload_cmds='$CC -r -o $output$reload_objs' hardcode_direct=no ;; motorola) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_direct=no #Motorola manual says yes, but my tests say they lie ;; esac runpath_var='LD_RUN_PATH' hardcode_shlibpath_var=no ;; sysv4.3*) archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_shlibpath_var=no export_dynamic_flag_spec='-Bexport' ;; sysv4*MP*) if test -d /usr/nec; then archive_cmds='$LD -G -h $soname -o $lib $libobjs $deplibs $linker_flags' hardcode_shlibpath_var=no runpath_var=LD_RUN_PATH hardcode_runpath_var=yes ld_shlibs=yes fi ;; sysv4*uw2* | sysv5OpenUNIX* | sysv5UnixWare7.[01].[10]* | unixware7* | sco3.2v5.0.[024]*) no_undefined_flag='$wl-z,text' archive_cmds_need_lc=no hardcode_shlibpath_var=no runpath_var='LD_RUN_PATH' if test yes = "$GCC"; then archive_cmds='$CC -shared $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' archive_expsym_cmds='$CC -shared $wl-Bexport:$export_symbols $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' else archive_cmds='$CC -G $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' archive_expsym_cmds='$CC -G $wl-Bexport:$export_symbols $wl-h,$soname -o $lib $libobjs $deplibs $compiler_flags' fi ;; sysv5* | sco3.2v5* | sco5v6*) # Note: We CANNOT use -z defs as we might desire, because we do not # link with -lc, and that would cause any symbols used from libc to # always be unresolved, which means just about no library would # ever link correctly. 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# This must be glibc/ELF. linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' finish_cmds='PATH="\$PATH:/sbin" ldconfig -n $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no # Some binutils ld are patched to set DT_RUNPATH if ${lt_cv_shlibpath_overrides_runpath+:} false; then : $as_echo_n "(cached) " >&6 else lt_cv_shlibpath_overrides_runpath=no save_LDFLAGS=$LDFLAGS save_libdir=$libdir eval "libdir=/foo; wl=\"$lt_prog_compiler_wl\"; \ LDFLAGS=\"\$LDFLAGS $hardcode_libdir_flag_spec\"" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ int main () { ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : if ($OBJDUMP -p conftest$ac_exeext) 2>/dev/null | grep "RUNPATH.*$libdir" >/dev/null; then : lt_cv_shlibpath_overrides_runpath=yes fi fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LDFLAGS=$save_LDFLAGS libdir=$save_libdir fi shlibpath_overrides_runpath=$lt_cv_shlibpath_overrides_runpath # This implies no fast_install, which is unacceptable. # Some rework will be needed to allow for fast_install # before this can be enabled. hardcode_into_libs=yes # Ideally, we could use ldconfig to report *all* directores which are # searched for libraries, however this is still not possible. Aside from not # being certain /sbin/ldconfig is available, command # 'ldconfig -N -X -v | grep ^/' on 64bit Fedora does not report /usr/lib64, # even though it is searched at run-time. Try to do the best guess by # appending ld.so.conf contents (and includes) to the search path. if test -f /etc/ld.so.conf; then lt_ld_extra=`awk '/^include / { system(sprintf("cd /etc; cat %s 2>/dev/null", \$2)); skip = 1; } { if (!skip) print \$0; skip = 0; }' < /etc/ld.so.conf | $SED -e 's/#.*//;/^[ ]*hwcap[ ]/d;s/[:, ]/ /g;s/=[^=]*$//;s/=[^= ]* / /g;s/"//g;/^$/d' | tr '\n' ' '` sys_lib_dlsearch_path_spec="/lib /usr/lib $lt_ld_extra" fi # We used to test for /lib/ld.so.1 and disable shared libraries on # powerpc, because MkLinux only supported shared libraries with the # GNU dynamic linker. Since this was broken with cross compilers, # most powerpc-linux boxes support dynamic linking these days and # people can always --disable-shared, the test was removed, and we # assume the GNU/Linux dynamic linker is in use. dynamic_linker='GNU/Linux ld.so' ;; netbsd*) version_type=sunos need_lib_prefix=no need_version=no if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/sbin" ldconfig -m $libdir' dynamic_linker='NetBSD (a.out) ld.so' else library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' dynamic_linker='NetBSD ld.elf_so' fi shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes ;; newsos6) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes ;; *nto* | *qnx*) version_type=qnx need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes dynamic_linker='ldqnx.so' ;; openbsd* | bitrig*) version_type=sunos sys_lib_dlsearch_path_spec=/usr/lib need_lib_prefix=no if test -z "`echo __ELF__ | $CC -E - | $GREP __ELF__`"; then need_version=no else need_version=yes fi library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/sbin" ldconfig -m $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes ;; os2*) libname_spec='$name' version_type=windows shrext_cmds=.dll need_version=no need_lib_prefix=no # OS/2 can only load a DLL with a base name of 8 characters or less. soname_spec='`test -n "$os2dllname" && libname="$os2dllname"; v=$($ECHO $release$versuffix | tr -d .-); n=$($ECHO $libname | cut -b -$((8 - ${#v})) | tr . _); $ECHO $n$v`$shared_ext' library_names_spec='${libname}_dll.$libext' dynamic_linker='OS/2 ld.exe' shlibpath_var=BEGINLIBPATH sys_lib_search_path_spec="/lib /usr/lib /usr/local/lib" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec postinstall_cmds='base_file=`basename \$file`~ dlpath=`$SHELL 2>&1 -c '\''. $dir/'\''\$base_file'\''i; $ECHO \$dlname'\''`~ dldir=$destdir/`dirname \$dlpath`~ test -d \$dldir || mkdir -p \$dldir~ $install_prog $dir/$dlname \$dldir/$dlname~ chmod a+x \$dldir/$dlname~ if test -n '\''$stripme'\'' && test -n '\''$striplib'\''; then eval '\''$striplib \$dldir/$dlname'\'' || exit \$?; fi' postuninstall_cmds='dldll=`$SHELL 2>&1 -c '\''. $file; $ECHO \$dlname'\''`~ dlpath=$dir/\$dldll~ $RM \$dlpath' ;; osf3* | osf4* | osf5*) version_type=osf need_lib_prefix=no need_version=no soname_spec='$libname$release$shared_ext$major' library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH sys_lib_search_path_spec="/usr/shlib /usr/ccs/lib /usr/lib/cmplrs/cc /usr/lib /usr/local/lib /var/shlib" sys_lib_dlsearch_path_spec=$sys_lib_search_path_spec ;; rdos*) dynamic_linker=no ;; solaris*) version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes # ldd complains unless libraries are executable postinstall_cmds='chmod +x $lib' ;; sunos4*) version_type=sunos library_names_spec='$libname$release$shared_ext$versuffix $libname$shared_ext$versuffix' finish_cmds='PATH="\$PATH:/usr/etc" ldconfig $libdir' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes if test yes = "$with_gnu_ld"; then need_lib_prefix=no fi need_version=yes ;; sysv4 | sysv4.3*) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH case $host_vendor in sni) shlibpath_overrides_runpath=no need_lib_prefix=no runpath_var=LD_RUN_PATH ;; siemens) need_lib_prefix=no ;; motorola) need_lib_prefix=no need_version=no shlibpath_overrides_runpath=no sys_lib_search_path_spec='/lib /usr/lib /usr/ccs/lib' ;; esac ;; sysv4*MP*) if test -d /usr/nec; then version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$shared_ext.$versuffix $libname$shared_ext.$major $libname$shared_ext' soname_spec='$libname$shared_ext.$major' shlibpath_var=LD_LIBRARY_PATH fi ;; sysv5* | sco3.2v5* | sco5v6* | unixware* | OpenUNIX* | sysv4*uw2*) version_type=sco need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes hardcode_into_libs=yes if test yes = "$with_gnu_ld"; then sys_lib_search_path_spec='/usr/local/lib /usr/gnu/lib /usr/ccs/lib /usr/lib /lib' else sys_lib_search_path_spec='/usr/ccs/lib /usr/lib' case $host_os in sco3.2v5*) sys_lib_search_path_spec="$sys_lib_search_path_spec /lib" ;; esac fi sys_lib_dlsearch_path_spec='/usr/lib' ;; tpf*) # TPF is a cross-target only. Preferred cross-host = GNU/Linux. version_type=linux # correct to gnu/linux during the next big refactor need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=no hardcode_into_libs=yes ;; uts4*) version_type=linux # correct to gnu/linux during the next big refactor library_names_spec='$libname$release$shared_ext$versuffix $libname$release$shared_ext$major $libname$shared_ext' soname_spec='$libname$release$shared_ext$major' shlibpath_var=LD_LIBRARY_PATH ;; *) dynamic_linker=no ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: result: $dynamic_linker" >&5 $as_echo "$dynamic_linker" >&6; } test no = "$dynamic_linker" && can_build_shared=no variables_saved_for_relink="PATH $shlibpath_var $runpath_var" if test yes = "$GCC"; then variables_saved_for_relink="$variables_saved_for_relink GCC_EXEC_PREFIX COMPILER_PATH LIBRARY_PATH" fi if test set = "${lt_cv_sys_lib_search_path_spec+set}"; then sys_lib_search_path_spec=$lt_cv_sys_lib_search_path_spec fi if test set = "${lt_cv_sys_lib_dlsearch_path_spec+set}"; then sys_lib_dlsearch_path_spec=$lt_cv_sys_lib_dlsearch_path_spec fi # remember unaugmented sys_lib_dlsearch_path content for libtool script decls... configure_time_dlsearch_path=$sys_lib_dlsearch_path_spec # ... but it needs LT_SYS_LIBRARY_PATH munging for other configure-time code func_munge_path_list sys_lib_dlsearch_path_spec "$LT_SYS_LIBRARY_PATH" # to be used as default LT_SYS_LIBRARY_PATH value in generated libtool configure_time_lt_sys_library_path=$LT_SYS_LIBRARY_PATH { $as_echo "$as_me:${as_lineno-$LINENO}: checking how to hardcode library paths into programs" >&5 $as_echo_n "checking how to hardcode library paths into programs... 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" >&6; } if ${ac_cv_lib_dl_dlopen+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-ldl $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char dlopen (); int main () { return dlopen (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_dl_dlopen=yes else ac_cv_lib_dl_dlopen=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_dl_dlopen" >&5 $as_echo "$ac_cv_lib_dl_dlopen" >&6; } if test "x$ac_cv_lib_dl_dlopen" = xyes; then : lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-ldl else lt_cv_dlopen=dyld lt_cv_dlopen_libs= lt_cv_dlopen_self=yes fi ;; tpf*) # Don't try to run any link tests for TPF. We know it's impossible # because TPF is a cross-compiler, and we know how we open DSOs. lt_cv_dlopen=dlopen lt_cv_dlopen_libs= lt_cv_dlopen_self=no ;; *) ac_fn_c_check_func "$LINENO" "shl_load" "ac_cv_func_shl_load" if test "x$ac_cv_func_shl_load" = xyes; then : lt_cv_dlopen=shl_load else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for shl_load in -ldld" >&5 $as_echo_n "checking for shl_load in -ldld... " >&6; } if ${ac_cv_lib_dld_shl_load+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-ldld $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char shl_load (); int main () { return shl_load (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_dld_shl_load=yes else ac_cv_lib_dld_shl_load=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_dld_shl_load" >&5 $as_echo "$ac_cv_lib_dld_shl_load" >&6; } if test "x$ac_cv_lib_dld_shl_load" = xyes; then : lt_cv_dlopen=shl_load lt_cv_dlopen_libs=-ldld else ac_fn_c_check_func "$LINENO" "dlopen" "ac_cv_func_dlopen" if test "x$ac_cv_func_dlopen" = xyes; then : lt_cv_dlopen=dlopen else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for dlopen in -ldl" >&5 $as_echo_n "checking for dlopen in -ldl... " >&6; } if ${ac_cv_lib_dl_dlopen+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-ldl $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char dlopen (); int main () { return dlopen (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_dl_dlopen=yes else ac_cv_lib_dl_dlopen=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_dl_dlopen" >&5 $as_echo "$ac_cv_lib_dl_dlopen" >&6; } if test "x$ac_cv_lib_dl_dlopen" = xyes; then : lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-ldl else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for dlopen in -lsvld" >&5 $as_echo_n "checking for dlopen in -lsvld... " >&6; } if ${ac_cv_lib_svld_dlopen+:} false; then : $as_echo_n "(cached) " >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lsvld $LIBS" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char dlopen (); int main () { return dlopen (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : ac_cv_lib_svld_dlopen=yes else ac_cv_lib_svld_dlopen=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_lib_svld_dlopen" >&5 $as_echo "$ac_cv_lib_svld_dlopen" >&6; } if test "x$ac_cv_lib_svld_dlopen" = xyes; then : lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-lsvld else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for dld_link in -ldld" >&5 $as_echo_n "checking for dld_link in -ldld... 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REPLACE_VFPRINTF=0; REPLACE_VPRINTF=0; REPLACE_VSNPRINTF=0; REPLACE_VSPRINTF=0; ac_fn_c_check_decl "$LINENO" "getdelim" "ac_cv_have_decl_getdelim" "$ac_includes_default" if test "x$ac_cv_have_decl_getdelim" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETDELIM $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "getline" "ac_cv_have_decl_getline" "$ac_includes_default" if test "x$ac_cv_have_decl_getline" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETLINE $ac_have_decl _ACEOF GNULIB_CHDIR=0; GNULIB_CHOWN=0; GNULIB_CLOSE=0; GNULIB_DUP=0; GNULIB_DUP2=0; GNULIB_DUP3=0; GNULIB_ENVIRON=0; GNULIB_EUIDACCESS=0; GNULIB_FACCESSAT=0; GNULIB_FCHDIR=0; GNULIB_FCHOWNAT=0; GNULIB_FDATASYNC=0; GNULIB_FSYNC=0; GNULIB_FTRUNCATE=0; GNULIB_GETCWD=0; GNULIB_GETDOMAINNAME=0; GNULIB_GETDTABLESIZE=0; GNULIB_GETGROUPS=0; GNULIB_GETHOSTNAME=0; GNULIB_GETLOGIN=0; GNULIB_GETLOGIN_R=0; GNULIB_GETPAGESIZE=0; GNULIB_GETUSERSHELL=0; GNULIB_GROUP_MEMBER=0; GNULIB_ISATTY=0; GNULIB_LCHOWN=0; GNULIB_LINK=0; GNULIB_LINKAT=0; GNULIB_LSEEK=0; GNULIB_PIPE=0; GNULIB_PIPE2=0; GNULIB_PREAD=0; GNULIB_PWRITE=0; GNULIB_READ=0; GNULIB_READLINK=0; GNULIB_READLINKAT=0; GNULIB_RMDIR=0; GNULIB_SETHOSTNAME=0; GNULIB_SLEEP=0; GNULIB_SYMLINK=0; GNULIB_SYMLINKAT=0; GNULIB_TRUNCATE=0; GNULIB_TTYNAME_R=0; GNULIB_UNISTD_H_NONBLOCKING=0; GNULIB_UNISTD_H_SIGPIPE=0; GNULIB_UNLINK=0; GNULIB_UNLINKAT=0; GNULIB_USLEEP=0; GNULIB_WRITE=0; HAVE_CHOWN=1; HAVE_DUP2=1; HAVE_DUP3=1; HAVE_EUIDACCESS=1; HAVE_FACCESSAT=1; HAVE_FCHDIR=1; HAVE_FCHOWNAT=1; HAVE_FDATASYNC=1; HAVE_FSYNC=1; HAVE_FTRUNCATE=1; HAVE_GETDTABLESIZE=1; HAVE_GETGROUPS=1; HAVE_GETHOSTNAME=1; HAVE_GETLOGIN=1; HAVE_GETPAGESIZE=1; HAVE_GROUP_MEMBER=1; HAVE_LCHOWN=1; HAVE_LINK=1; HAVE_LINKAT=1; HAVE_PIPE=1; HAVE_PIPE2=1; HAVE_PREAD=1; HAVE_PWRITE=1; HAVE_READLINK=1; HAVE_READLINKAT=1; HAVE_SETHOSTNAME=1; HAVE_SLEEP=1; HAVE_SYMLINK=1; HAVE_SYMLINKAT=1; HAVE_TRUNCATE=1; HAVE_UNLINKAT=1; HAVE_USLEEP=1; HAVE_DECL_ENVIRON=1; HAVE_DECL_FCHDIR=1; HAVE_DECL_FDATASYNC=1; HAVE_DECL_GETDOMAINNAME=1; HAVE_DECL_GETLOGIN=1; HAVE_DECL_GETLOGIN_R=1; HAVE_DECL_GETPAGESIZE=1; HAVE_DECL_GETUSERSHELL=1; HAVE_DECL_SETHOSTNAME=1; HAVE_DECL_TTYNAME_R=1; HAVE_OS_H=0; HAVE_SYS_PARAM_H=0; REPLACE_CHOWN=0; REPLACE_CLOSE=0; REPLACE_DUP=0; REPLACE_DUP2=0; REPLACE_FACCESSAT=0; REPLACE_FCHOWNAT=0; REPLACE_FTRUNCATE=0; REPLACE_GETCWD=0; REPLACE_GETDOMAINNAME=0; REPLACE_GETDTABLESIZE=0; REPLACE_GETLOGIN_R=0; REPLACE_GETGROUPS=0; REPLACE_GETPAGESIZE=0; REPLACE_ISATTY=0; REPLACE_LCHOWN=0; REPLACE_LINK=0; REPLACE_LINKAT=0; REPLACE_LSEEK=0; REPLACE_PREAD=0; REPLACE_PWRITE=0; REPLACE_READ=0; REPLACE_READLINK=0; REPLACE_READLINKAT=0; REPLACE_RMDIR=0; REPLACE_SLEEP=0; REPLACE_SYMLINK=0; REPLACE_SYMLINKAT=0; REPLACE_TRUNCATE=0; REPLACE_TTYNAME_R=0; REPLACE_UNLINK=0; REPLACE_UNLINKAT=0; REPLACE_USLEEP=0; REPLACE_WRITE=0; UNISTD_H_HAVE_WINSOCK2_H=0; UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=0; if test $gl_cv_have_include_next = yes; then gl_cv_next_getopt_h='<'getopt.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_getopt_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_getopt_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'getopt.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_getopt_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_getopt_h gl_cv_next_getopt_h='"'$gl_header'"' else gl_cv_next_getopt_h='<'getopt.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_getopt_h" >&5 $as_echo "$gl_cv_next_getopt_h" >&6; } fi NEXT_GETOPT_H=$gl_cv_next_getopt_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'getopt.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_getopt_h fi NEXT_AS_FIRST_DIRECTIVE_GETOPT_H=$gl_next_as_first_directive if test $ac_cv_header_getopt_h = yes; then HAVE_GETOPT_H=1 else HAVE_GETOPT_H=0 fi gl_replace_getopt= if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then for ac_header in getopt.h do : ac_fn_c_check_header_mongrel "$LINENO" "getopt.h" "ac_cv_header_getopt_h" "$ac_includes_default" if test "x$ac_cv_header_getopt_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_GETOPT_H 1 _ACEOF else gl_replace_getopt=yes fi done fi if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then for ac_func in getopt_long_only do : ac_fn_c_check_func "$LINENO" "getopt_long_only" "ac_cv_func_getopt_long_only" if test "x$ac_cv_func_getopt_long_only" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_GETOPT_LONG_ONLY 1 _ACEOF else gl_replace_getopt=yes fi done fi if test -z "$gl_replace_getopt"; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether getopt is POSIX compatible" >&5 $as_echo_n "checking whether getopt is POSIX compatible... " >&6; } if ${gl_cv_func_getopt_posix+:} false; then : $as_echo_n "(cached) " >&6 else if test $cross_compiling = no; then if test "$cross_compiling" = yes; then : { { $as_echo "$as_me:${as_lineno-$LINENO}: error: in \`$ac_pwd':" >&5 $as_echo "$as_me: error: in \`$ac_pwd':" >&2;} as_fn_error $? "cannot run test program while cross compiling See \`config.log' for more details" "$LINENO" 5; } else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { static char program[] = "program"; static char a[] = "-a"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, a, foo, bar, NULL }; int c; c = getopt (4, argv, "ab"); if (!(c == 'a')) return 1; c = getopt (4, argv, "ab"); if (!(c == -1)) return 2; if (!(optind == 2)) return 3; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_posix=maybe else gl_cv_func_getopt_posix=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi if test $gl_cv_func_getopt_posix = maybe; then if test "$cross_compiling" = yes; then : { { $as_echo "$as_me:${as_lineno-$LINENO}: error: in \`$ac_pwd':" >&5 $as_echo "$as_me: error: in \`$ac_pwd':" >&2;} as_fn_error $? "cannot run test program while cross compiling See \`config.log' for more details" "$LINENO" 5; } else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { static char program[] = "program"; static char donald[] = "donald"; static char p[] = "-p"; static char billy[] = "billy"; static char duck[] = "duck"; static char a[] = "-a"; static char bar[] = "bar"; char *argv[] = { program, donald, p, billy, duck, a, bar, NULL }; int c; c = getopt (7, argv, "+abp:q:"); if (!(c == -1)) return 4; if (!(strcmp (argv[0], "program") == 0)) return 5; if (!(strcmp (argv[1], "donald") == 0)) return 6; if (!(strcmp (argv[2], "-p") == 0)) return 7; if (!(strcmp (argv[3], "billy") == 0)) return 8; if (!(strcmp (argv[4], "duck") == 0)) return 9; if (!(strcmp (argv[5], "-a") == 0)) return 10; if (!(strcmp (argv[6], "bar") == 0)) return 11; if (!(optind == 1)) return 12; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_posix=maybe else gl_cv_func_getopt_posix=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi if test $gl_cv_func_getopt_posix = maybe; then if test "$cross_compiling" = yes; then : { { $as_echo "$as_me:${as_lineno-$LINENO}: error: in \`$ac_pwd':" >&5 $as_echo "$as_me: error: in \`$ac_pwd':" >&2;} as_fn_error $? "cannot run test program while cross compiling See \`config.log' for more details" "$LINENO" 5; } else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { static char program[] = "program"; static char ab[] = "-ab"; char *argv[3] = { program, ab, NULL }; if (getopt (2, argv, "ab:") != 'a') return 13; if (getopt (2, argv, "ab:") != '?') return 14; if (optopt != 'b') return 15; if (optind != 2) return 16; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_posix=yes else gl_cv_func_getopt_posix=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi else case "$host_os" in darwin* | aix* | mingw*) gl_cv_func_getopt_posix="guessing no";; *) gl_cv_func_getopt_posix="guessing yes";; esac fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getopt_posix" >&5 $as_echo "$gl_cv_func_getopt_posix" >&6; } case "$gl_cv_func_getopt_posix" in *no) gl_replace_getopt=yes ;; esac fi if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working GNU getopt function" >&5 $as_echo_n "checking for working GNU getopt function... " >&6; } if ${gl_cv_func_getopt_gnu+:} false; then : $as_echo_n "(cached) " >&6 else # Even with POSIXLY_CORRECT, the GNU extension of leading '-' in the # optstring is necessary for programs like m4 that have POSIX-mandated # semantics for supporting options interspersed with files. # Also, since getopt_long is a GNU extension, we require optind=0. # Bash ties 'set -o posix' to a non-exported POSIXLY_CORRECT; # so take care to revert to the correct (non-)export state. gl_awk_probe='BEGIN { if ("POSIXLY_CORRECT" in ENVIRON) print "x" }' case ${POSIXLY_CORRECT+x}`$AWK "$gl_awk_probe" conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #if defined __MACH__ && defined __APPLE__ /* Avoid a crash on Mac OS X. */ #include #include #include #include #include #include /* The exception port on which our thread listens. */ static mach_port_t our_exception_port; /* The main function of the thread listening for exceptions of type EXC_BAD_ACCESS. */ static void * mach_exception_thread (void *arg) { /* Buffer for a message to be received. */ struct { mach_msg_header_t head; mach_msg_body_t msgh_body; char data[1024]; } msg; mach_msg_return_t retval; /* Wait for a message on the exception port. */ retval = mach_msg (&msg.head, MACH_RCV_MSG | MACH_RCV_LARGE, 0, sizeof (msg), our_exception_port, MACH_MSG_TIMEOUT_NONE, MACH_PORT_NULL); if (retval != MACH_MSG_SUCCESS) abort (); exit (1); } static void nocrash_init (void) { mach_port_t self = mach_task_self (); /* Allocate a port on which the thread shall listen for exceptions. */ if (mach_port_allocate (self, MACH_PORT_RIGHT_RECEIVE, &our_exception_port) == KERN_SUCCESS) { /* See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/mach_port_insert_right.html. */ if (mach_port_insert_right (self, our_exception_port, our_exception_port, MACH_MSG_TYPE_MAKE_SEND) == KERN_SUCCESS) { /* The exceptions we want to catch. Only EXC_BAD_ACCESS is interesting for us. */ exception_mask_t mask = EXC_MASK_BAD_ACCESS; /* Create the thread listening on the exception port. */ pthread_attr_t attr; pthread_t thread; if (pthread_attr_init (&attr) == 0 && pthread_attr_setdetachstate (&attr, PTHREAD_CREATE_DETACHED) == 0 && pthread_create (&thread, &attr, mach_exception_thread, NULL) == 0) { pthread_attr_destroy (&attr); /* Replace the exception port info for these exceptions with our own. Note that we replace the exception port for the entire task, not only for a particular thread. This has the effect that when our exception port gets the message, the thread specific exception port has already been asked, and we don't need to bother about it. See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/task_set_exception_ports.html. */ task_set_exception_ports (self, mask, our_exception_port, EXCEPTION_DEFAULT, MACHINE_THREAD_STATE); } } } } #elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Avoid a crash on native Windows. */ #define WIN32_LEAN_AND_MEAN #include #include static LONG WINAPI exception_filter (EXCEPTION_POINTERS *ExceptionInfo) { switch (ExceptionInfo->ExceptionRecord->ExceptionCode) { case EXCEPTION_ACCESS_VIOLATION: case EXCEPTION_IN_PAGE_ERROR: case EXCEPTION_STACK_OVERFLOW: case EXCEPTION_GUARD_PAGE: case EXCEPTION_PRIV_INSTRUCTION: case EXCEPTION_ILLEGAL_INSTRUCTION: case EXCEPTION_DATATYPE_MISALIGNMENT: case EXCEPTION_ARRAY_BOUNDS_EXCEEDED: case EXCEPTION_NONCONTINUABLE_EXCEPTION: exit (1); } return EXCEPTION_CONTINUE_SEARCH; } static void nocrash_init (void) { SetUnhandledExceptionFilter ((LPTOP_LEVEL_EXCEPTION_FILTER) exception_filter); } #else /* Avoid a crash on POSIX systems. */ #include #include /* A POSIX signal handler. */ static void exception_handler (int sig) { _exit (1); } static void nocrash_init (void) { #ifdef SIGSEGV signal (SIGSEGV, exception_handler); #endif #ifdef SIGBUS signal (SIGBUS, exception_handler); #endif } #endif int main () { int result = 0; nocrash_init(); /* This code succeeds on glibc 2.8, OpenBSD 4.0, Cygwin, mingw, and fails on Mac OS X 10.5, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10. */ { static char conftest[] = "conftest"; static char plus[] = "-+"; char *argv[3] = { conftest, plus, NULL }; opterr = 0; if (getopt (2, argv, "+a") != '?') result |= 1; } /* This code succeeds on glibc 2.8, mingw, and fails on Mac OS X 10.5, OpenBSD 4.0, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10, Cygwin 1.5.x. */ { static char program[] = "program"; static char p[] = "-p"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, p, foo, bar, NULL }; optind = 1; if (getopt (4, argv, "p::") != 'p') result |= 2; else if (optarg != NULL) result |= 4; else if (getopt (4, argv, "p::") != -1) result |= 6; else if (optind != 2) result |= 8; } /* This code succeeds on glibc 2.8 and fails on Cygwin 1.7.0. */ { static char program[] = "program"; static char foo[] = "foo"; static char p[] = "-p"; char *argv[] = { program, foo, p, NULL }; optind = 0; if (getopt (3, argv, "-p") != 1) result |= 16; else if (getopt (3, argv, "-p") != 'p') result |= 16; } /* This code fails on glibc 2.11. */ { static char program[] = "program"; static char b[] = "-b"; static char a[] = "-a"; char *argv[] = { program, b, a, NULL }; optind = opterr = 0; if (getopt (3, argv, "+:a:b") != 'b') result |= 32; else if (getopt (3, argv, "+:a:b") != ':') result |= 32; } /* This code dumps core on glibc 2.14. */ { static char program[] = "program"; static char w[] = "-W"; static char dummy[] = "dummy"; char *argv[] = { program, w, dummy, NULL }; optind = opterr = 1; if (getopt (3, argv, "W;") != 'W') result |= 64; } return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_gnu=yes else gl_cv_func_getopt_gnu=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi case $gl_had_POSIXLY_CORRECT in exported) ;; yes) { POSIXLY_CORRECT=; unset POSIXLY_CORRECT;}; POSIXLY_CORRECT=1 ;; *) { POSIXLY_CORRECT=; unset POSIXLY_CORRECT;} ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getopt_gnu" >&5 $as_echo "$gl_cv_func_getopt_gnu" >&6; } if test "$gl_cv_func_getopt_gnu" != yes; then gl_replace_getopt=yes else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working GNU getopt_long function" >&5 $as_echo_n "checking for working GNU getopt_long function... " >&6; } if ${gl_cv_func_getopt_long_gnu+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in openbsd*) gl_cv_func_getopt_long_gnu="guessing no";; *) gl_cv_func_getopt_long_gnu="guessing yes";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include int main () { static const struct option long_options[] = { { "xtremely-",no_argument, NULL, 1003 }, { "xtra", no_argument, NULL, 1001 }, { "xtreme", no_argument, NULL, 1002 }, { "xtremely", no_argument, NULL, 1003 }, { NULL, 0, NULL, 0 } }; /* This code fails on OpenBSD 5.0. */ { static char program[] = "program"; static char xtremel[] = "--xtremel"; char *argv[] = { program, xtremel, NULL }; int option_index; optind = 1; opterr = 0; if (getopt_long (2, argv, "", long_options, &option_index) != 1003) return 1; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getopt_long_gnu=yes else gl_cv_func_getopt_long_gnu=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getopt_long_gnu" >&5 $as_echo "$gl_cv_func_getopt_long_gnu" >&6; } case "$gl_cv_func_getopt_long_gnu" in *yes) ;; *) gl_replace_getopt=yes ;; esac fi fi cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef _MSC_VER MicrosoftCompiler #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "MicrosoftCompiler" >/dev/null 2>&1; then : gl_asmext='asm' gl_c_asm_opt='-c -Fa' else gl_asmext='s' gl_c_asm_opt='-S' fi rm -f conftest* { $as_echo "$as_me:${as_lineno-$LINENO}: checking host CPU and C ABI" >&5 $as_echo_n "checking host CPU and C ABI... " >&6; } if ${gl_cv_host_cpu_c_abi+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_cpu" in i[4567]86 ) gl_cv_host_cpu_c_abi=i386 ;; x86_64 ) # On x86_64 systems, the C compiler may be generating code in one of # these ABIs: # - 64-bit instruction set, 64-bit pointers, 64-bit 'long': x86_64. # - 64-bit instruction set, 64-bit pointers, 32-bit 'long': x86_64 # with native Windows (mingw, MSVC). # - 64-bit instruction set, 32-bit pointers, 32-bit 'long': x86_64-x32. # - 32-bit instruction set, 32-bit pointers, 32-bit 'long': i386. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if (defined __x86_64__ || defined __amd64__ \ || defined _M_X64 || defined _M_AMD64) int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined __ILP32__ || defined _ILP32 int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=x86_64-x32 else gl_cv_host_cpu_c_abi=x86_64 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else gl_cv_host_cpu_c_abi=i386 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; alphaev[4-8] | alphaev56 | alphapca5[67] | alphaev6[78] ) gl_cv_host_cpu_c_abi=alpha ;; arm* | aarch64 ) # Assume arm with EABI. # On arm64 systems, the C compiler may be generating code in one of # these ABIs: # - aarch64 instruction set, 64-bit pointers, 64-bit 'long': arm64. # - aarch64 instruction set, 32-bit pointers, 32-bit 'long': arm64-ilp32. # - 32-bit instruction set, 32-bit pointers, 32-bit 'long': arm or armhf. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __aarch64__ int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined __ILP32__ || defined _ILP32 int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=arm64-ilp32 else gl_cv_host_cpu_c_abi=arm64 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else # Don't distinguish little-endian and big-endian arm, since they # don't require different machine code for simple operations and # since the user can distinguish them through the preprocessor # defines __ARMEL__ vs. __ARMEB__. # But distinguish arm which passes floating-point arguments and # return values in integer registers (r0, r1, ...) - this is # gcc -mfloat-abi=soft or gcc -mfloat-abi=softfp - from arm which # passes them in float registers (s0, s1, ...) and double registers # (d0, d1, ...) - this is gcc -mfloat-abi=hard. GCC 4.6 or newer # sets the preprocessor defines __ARM_PCS (for the first case) and # __ARM_PCS_VFP (for the second case), but older GCC does not. echo 'double ddd; void func (double dd) { ddd = dd; }' > conftest.c # Look for a reference to the register d0 in the .s file. { ac_try='${CC-cc} $CFLAGS $CPPFLAGS $gl_c_asm_opt conftest.c' { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_try\""; } >&5 (eval $ac_try) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; }; } >/dev/null 2>&1 if LC_ALL=C grep -E 'd0,' conftest.$gl_asmext >/dev/null; then gl_cv_host_cpu_c_abi=armhf else gl_cv_host_cpu_c_abi=arm fi rm -f conftest* fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; hppa1.0 | hppa1.1 | hppa2.0* | hppa64 ) # On hppa, the C compiler may be generating 32-bit code or 64-bit # code. In the latter case, it defines _LP64 and __LP64__. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __LP64__ int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=hppa64 else gl_cv_host_cpu_c_abi=hppa fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; ia64* ) # On ia64 on HP-UX, the C compiler may be generating 64-bit code or # 32-bit code. In the latter case, it defines _ILP32. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef _ILP32 int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=ia64-ilp32 else gl_cv_host_cpu_c_abi=ia64 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; mips* ) # We should also check for (_MIPS_SZPTR == 64), but gcc keeps this # at 32. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined _MIPS_SZLONG && (_MIPS_SZLONG == 64) int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=mips64 else # In the n32 ABI, _ABIN32 is defined, _ABIO32 is not defined (but # may later get defined by ), and _MIPS_SIM == _ABIN32. # In the 32 ABI, _ABIO32 is defined, _ABIN32 is not defined (but # may later get defined by ), and _MIPS_SIM == _ABIO32. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if (_MIPS_SIM == _ABIN32) int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=mipsn32 else gl_cv_host_cpu_c_abi=mips fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; powerpc* ) # Different ABIs are in use on AIX vs. Mac OS X vs. Linux,*BSD. # No need to distinguish them here; the caller may distinguish # them based on the OS. # On powerpc64 systems, the C compiler may still be generating # 32-bit code. And on powerpc-ibm-aix systems, the C compiler may # be generating 64-bit code. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined __powerpc64__ || defined _ARCH_PPC64 int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # On powerpc64, there are two ABIs on Linux: The AIX compatible # one and the ELFv2 one. The latter defines _CALL_ELF=2. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined _CALL_ELF && _CALL_ELF == 2 int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=powerpc64-elfv2 else gl_cv_host_cpu_c_abi=powerpc64 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else gl_cv_host_cpu_c_abi=powerpc fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; rs6000 ) gl_cv_host_cpu_c_abi=powerpc ;; s390* ) # On s390x, the C compiler may be generating 64-bit (= s390x) code # or 31-bit (= s390) code. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined __LP64__ || defined __s390x__ int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=s390x else gl_cv_host_cpu_c_abi=s390 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; sparc | sparc64 ) # UltraSPARCs running Linux have `uname -m` = "sparc64", but the # C compiler still generates 32-bit code. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined __sparcv9 || defined __arch64__ int ok; #else error fail #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_host_cpu_c_abi=sparc64 else gl_cv_host_cpu_c_abi=sparc fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ;; *) gl_cv_host_cpu_c_abi="$host_cpu" ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_host_cpu_c_abi" >&5 $as_echo "$gl_cv_host_cpu_c_abi" >&6; } HOST_CPU=`echo "$gl_cv_host_cpu_c_abi" | sed -e 's/-.*//'` HOST_CPU_C_ABI="$gl_cv_host_cpu_c_abi" # This was # AC_DEFINE_UNQUOTED([__${HOST_CPU}__]) # AC_DEFINE_UNQUOTED([__${HOST_CPU_C_ABI}__]) # earlier, but KAI C++ 3.2d doesn't like this. sed -e 's/-/_/g' >> confdefs.h <' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_limits_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_limits_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'limits.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_limits_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_limits_h gl_cv_next_limits_h='"'$gl_header'"' else gl_cv_next_limits_h='<'limits.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_limits_h" >&5 $as_echo "$gl_cv_next_limits_h" >&6; } fi NEXT_LIMITS_H=$gl_cv_next_limits_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'limits.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_limits_h fi NEXT_AS_FIRST_DIRECTIVE_LIMITS_H=$gl_next_as_first_directive { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether limits.h has ULLONG_WIDTH etc." >&5 $as_echo_n "checking whether limits.h has ULLONG_WIDTH etc.... " >&6; } if ${gl_cv_header_limits_width+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include int ullw = ULLONG_WIDTH; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_limits_width=yes else gl_cv_header_limits_width=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_limits_width" >&5 $as_echo "$gl_cv_header_limits_width" >&6; } if test "$gl_cv_header_limits_width" = yes; then LIMITS_H= else LIMITS_H=limits.h fi if test -n "$LIMITS_H"; then GL_GENERATE_LIMITS_H_TRUE= GL_GENERATE_LIMITS_H_FALSE='#' else GL_GENERATE_LIMITS_H_TRUE='#' GL_GENERATE_LIMITS_H_FALSE= fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wint_t" >&5 $as_echo_n "checking for wint_t... " >&6; } if ${gt_cv_c_wint_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include wint_t foo = (wchar_t)'\0'; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_c_wint_t=yes else gt_cv_c_wint_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_c_wint_t" >&5 $as_echo "$gt_cv_c_wint_t" >&6; } if test $gt_cv_c_wint_t = yes; then $as_echo "#define HAVE_WINT_T 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether wint_t is too small" >&5 $as_echo_n "checking whether wint_t is too small... " >&6; } if ${gl_cv_type_wint_t_too_small+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include #endif #include int verify[sizeof (wint_t) < sizeof (int) ? -1 : 1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wint_t_too_small=no else gl_cv_type_wint_t_too_small=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wint_t_too_small" >&5 $as_echo "$gl_cv_type_wint_t_too_small" >&6; } if test $gl_cv_type_wint_t_too_small = yes; then GNULIB_OVERRIDES_WINT_T=1 else GNULIB_OVERRIDES_WINT_T=0 fi else GNULIB_OVERRIDES_WINT_T=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for unsigned long long int" >&5 $as_echo_n "checking for unsigned long long int... " >&6; } if ${ac_cv_type_unsigned_long_long_int+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_type_unsigned_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* For now, do not test the preprocessor; as of 2007 there are too many implementations with broken preprocessors. Perhaps this can be revisited in 2012. In the meantime, code should not expect #if to work with literals wider than 32 bits. */ /* Test literals. */ long long int ll = 9223372036854775807ll; long long int nll = -9223372036854775807LL; unsigned long long int ull = 18446744073709551615ULL; /* Test constant expressions. */ typedef int a[((-9223372036854775807LL < 0 && 0 < 9223372036854775807ll) ? 1 : -1)]; typedef int b[(18446744073709551615ULL <= (unsigned long long int) -1 ? 1 : -1)]; int i = 63; int main () { /* Test availability of runtime routines for shift and division. */ long long int llmax = 9223372036854775807ll; unsigned long long int ullmax = 18446744073709551615ull; return ((ll << 63) | (ll >> 63) | (ll < i) | (ll > i) | (llmax / ll) | (llmax % ll) | (ull << 63) | (ull >> 63) | (ull << i) | (ull >> i) | (ullmax / ull) | (ullmax % ull)); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : else ac_cv_type_unsigned_long_long_int=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_type_unsigned_long_long_int" >&5 $as_echo "$ac_cv_type_unsigned_long_long_int" >&6; } if test $ac_cv_type_unsigned_long_long_int = yes; then $as_echo "#define HAVE_UNSIGNED_LONG_LONG_INT 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for long long int" >&5 $as_echo_n "checking for long long int... " >&6; } if ${ac_cv_type_long_long_int+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_type_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then ac_cv_type_long_long_int=$ac_cv_type_unsigned_long_long_int if test $ac_cv_type_long_long_int = yes; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifndef LLONG_MAX # define HALF \ (1LL << (sizeof (long long int) * CHAR_BIT - 2)) # define LLONG_MAX (HALF - 1 + HALF) #endif int main () { long long int n = 1; int i; for (i = 0; ; i++) { long long int m = n << i; if (m >> i != n) return 1; if (LLONG_MAX / 2 < m) break; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : else ac_cv_type_long_long_int=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_type_long_long_int" >&5 $as_echo "$ac_cv_type_long_long_int" >&6; } if test $ac_cv_type_long_long_int = yes; then $as_echo "#define HAVE_LONG_LONG_INT 1" >>confdefs.h fi gl_cv_c_multiarch=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : arch= prev= for word in ${CC} ${CFLAGS} ${CPPFLAGS} ${LDFLAGS}; do if test -n "$prev"; then case $word in i?86 | x86_64 | ppc | ppc64) if test -z "$arch" || test "$arch" = "$word"; then arch="$word" else gl_cv_c_multiarch=yes fi ;; esac prev= else if test "x$word" = "x-arch"; then prev=arch fi fi done fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $gl_cv_c_multiarch = yes; then APPLE_UNIVERSAL_BUILD=1 else APPLE_UNIVERSAL_BUILD=0 fi if test $ac_cv_type_long_long_int = yes; then HAVE_LONG_LONG_INT=1 else HAVE_LONG_LONG_INT=0 fi if test $ac_cv_type_unsigned_long_long_int = yes; then HAVE_UNSIGNED_LONG_LONG_INT=1 else HAVE_UNSIGNED_LONG_LONG_INT=0 fi if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi if test $ac_cv_header_inttypes_h = yes; then HAVE_INTTYPES_H=1 else HAVE_INTTYPES_H=0 fi if test $ac_cv_header_sys_types_h = yes; then HAVE_SYS_TYPES_H=1 else HAVE_SYS_TYPES_H=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_stdint_h='<'stdint.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_stdint_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_stdint_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'stdint.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_stdint_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_stdint_h gl_cv_next_stdint_h='"'$gl_header'"' else gl_cv_next_stdint_h='<'stdint.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_stdint_h" >&5 $as_echo "$gl_cv_next_stdint_h" >&6; } fi NEXT_STDINT_H=$gl_cv_next_stdint_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'stdint.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_stdint_h fi NEXT_AS_FIRST_DIRECTIVE_STDINT_H=$gl_next_as_first_directive if test $ac_cv_header_stdint_h = yes; then HAVE_STDINT_H=1 else HAVE_STDINT_H=0 fi if test $ac_cv_header_stdint_h = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stdint.h conforms to C99" >&5 $as_echo_n "checking whether stdint.h conforms to C99... " >&6; } if ${gl_cv_header_working_stdint_h+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_header_working_stdint_h=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include /* Dragonfly defines WCHAR_MIN, WCHAR_MAX only in . */ #if !(defined WCHAR_MIN && defined WCHAR_MAX) #error "WCHAR_MIN, WCHAR_MAX not defined in " #endif /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif #ifdef INT8_MAX int8_t a1 = INT8_MAX; int8_t a1min = INT8_MIN; #endif #ifdef INT16_MAX int16_t a2 = INT16_MAX; int16_t a2min = INT16_MIN; #endif #ifdef INT32_MAX int32_t a3 = INT32_MAX; int32_t a3min = INT32_MIN; #endif #ifdef INT64_MAX int64_t a4 = INT64_MAX; int64_t a4min = INT64_MIN; #endif #ifdef UINT8_MAX uint8_t b1 = UINT8_MAX; #else typedef int b1[(unsigned char) -1 != 255 ? 1 : -1]; #endif #ifdef UINT16_MAX uint16_t b2 = UINT16_MAX; #endif #ifdef UINT32_MAX uint32_t b3 = UINT32_MAX; #endif #ifdef UINT64_MAX uint64_t b4 = UINT64_MAX; #endif int_least8_t c1 = INT8_C (0x7f); int_least8_t c1max = INT_LEAST8_MAX; int_least8_t c1min = INT_LEAST8_MIN; int_least16_t c2 = INT16_C (0x7fff); int_least16_t c2max = INT_LEAST16_MAX; int_least16_t c2min = INT_LEAST16_MIN; int_least32_t c3 = INT32_C (0x7fffffff); int_least32_t c3max = INT_LEAST32_MAX; int_least32_t c3min = INT_LEAST32_MIN; int_least64_t c4 = INT64_C (0x7fffffffffffffff); int_least64_t c4max = INT_LEAST64_MAX; int_least64_t c4min = INT_LEAST64_MIN; uint_least8_t d1 = UINT8_C (0xff); uint_least8_t d1max = UINT_LEAST8_MAX; uint_least16_t d2 = UINT16_C (0xffff); uint_least16_t d2max = UINT_LEAST16_MAX; uint_least32_t d3 = UINT32_C (0xffffffff); uint_least32_t d3max = UINT_LEAST32_MAX; uint_least64_t d4 = UINT64_C (0xffffffffffffffff); uint_least64_t d4max = UINT_LEAST64_MAX; int_fast8_t e1 = INT_FAST8_MAX; int_fast8_t e1min = INT_FAST8_MIN; int_fast16_t e2 = INT_FAST16_MAX; int_fast16_t e2min = INT_FAST16_MIN; int_fast32_t e3 = INT_FAST32_MAX; int_fast32_t e3min = INT_FAST32_MIN; int_fast64_t e4 = INT_FAST64_MAX; int_fast64_t e4min = INT_FAST64_MIN; uint_fast8_t f1 = UINT_FAST8_MAX; uint_fast16_t f2 = UINT_FAST16_MAX; uint_fast32_t f3 = UINT_FAST32_MAX; uint_fast64_t f4 = UINT_FAST64_MAX; #ifdef INTPTR_MAX intptr_t g = INTPTR_MAX; intptr_t gmin = INTPTR_MIN; #endif #ifdef UINTPTR_MAX uintptr_t h = UINTPTR_MAX; #endif intmax_t i = INTMAX_MAX; uintmax_t j = UINTMAX_MAX; /* Check that SIZE_MAX has the correct type, if possible. */ #if 201112 <= __STDC_VERSION__ int k = _Generic (SIZE_MAX, size_t: 0); #elif (2 <= __GNUC__ || defined __IBM__TYPEOF__ \ || (0x5110 <= __SUNPRO_C && !__STDC__)) extern size_t k; extern __typeof__ (SIZE_MAX) k; #endif #include /* for CHAR_BIT */ #define TYPE_MINIMUM(t) \ ((t) ((t) 0 < (t) -1 ? (t) 0 : ~ TYPE_MAXIMUM (t))) #define TYPE_MAXIMUM(t) \ ((t) ((t) 0 < (t) -1 \ ? (t) -1 \ : ((((t) 1 << (sizeof (t) * CHAR_BIT - 2)) - 1) * 2 + 1))) struct s { int check_PTRDIFF: PTRDIFF_MIN == TYPE_MINIMUM (ptrdiff_t) && PTRDIFF_MAX == TYPE_MAXIMUM (ptrdiff_t) ? 1 : -1; /* Detect bug in FreeBSD 6.0 / ia64. */ int check_SIG_ATOMIC: SIG_ATOMIC_MIN == TYPE_MINIMUM (sig_atomic_t) && SIG_ATOMIC_MAX == TYPE_MAXIMUM (sig_atomic_t) ? 1 : -1; int check_SIZE: SIZE_MAX == TYPE_MAXIMUM (size_t) ? 1 : -1; int check_WCHAR: WCHAR_MIN == TYPE_MINIMUM (wchar_t) && WCHAR_MAX == TYPE_MAXIMUM (wchar_t) ? 1 : -1; /* Detect bug in mingw. */ int check_WINT: WINT_MIN == TYPE_MINIMUM (wint_t) && WINT_MAX == TYPE_MAXIMUM (wint_t) ? 1 : -1; /* Detect bugs in glibc 2.4 and Solaris 10 stdint.h, among others. */ int check_UINT8_C: (-1 < UINT8_C (0)) == (-1 < (uint_least8_t) 0) ? 1 : -1; int check_UINT16_C: (-1 < UINT16_C (0)) == (-1 < (uint_least16_t) 0) ? 1 : -1; /* Detect bugs in OpenBSD 3.9 stdint.h. */ #ifdef UINT8_MAX int check_uint8: (uint8_t) -1 == UINT8_MAX ? 1 : -1; #endif #ifdef UINT16_MAX int check_uint16: (uint16_t) -1 == UINT16_MAX ? 1 : -1; #endif #ifdef UINT32_MAX int check_uint32: (uint32_t) -1 == UINT32_MAX ? 1 : -1; #endif #ifdef UINT64_MAX int check_uint64: (uint64_t) -1 == UINT64_MAX ? 1 : -1; #endif int check_uint_least8: (uint_least8_t) -1 == UINT_LEAST8_MAX ? 1 : -1; int check_uint_least16: (uint_least16_t) -1 == UINT_LEAST16_MAX ? 1 : -1; int check_uint_least32: (uint_least32_t) -1 == UINT_LEAST32_MAX ? 1 : -1; int check_uint_least64: (uint_least64_t) -1 == UINT_LEAST64_MAX ? 1 : -1; int check_uint_fast8: (uint_fast8_t) -1 == UINT_FAST8_MAX ? 1 : -1; int check_uint_fast16: (uint_fast16_t) -1 == UINT_FAST16_MAX ? 1 : -1; int check_uint_fast32: (uint_fast32_t) -1 == UINT_FAST32_MAX ? 1 : -1; int check_uint_fast64: (uint_fast64_t) -1 == UINT_FAST64_MAX ? 1 : -1; int check_uintptr: (uintptr_t) -1 == UINTPTR_MAX ? 1 : -1; int check_uintmax: (uintmax_t) -1 == UINTMAX_MAX ? 1 : -1; int check_size: (size_t) -1 == SIZE_MAX ? 1 : -1; }; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_header_working_stdint_h="guessing yes" ;; # In general, assume it works. *) gl_cv_header_working_stdint_h="guessing yes" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif #include #include #define MVAL(macro) MVAL1(macro) #define MVAL1(expression) #expression static const char *macro_values[] = { #ifdef INT8_MAX MVAL (INT8_MAX), #endif #ifdef INT16_MAX MVAL (INT16_MAX), #endif #ifdef INT32_MAX MVAL (INT32_MAX), #endif #ifdef INT64_MAX MVAL (INT64_MAX), #endif #ifdef UINT8_MAX MVAL (UINT8_MAX), #endif #ifdef UINT16_MAX MVAL (UINT16_MAX), #endif #ifdef UINT32_MAX MVAL (UINT32_MAX), #endif #ifdef UINT64_MAX MVAL (UINT64_MAX), #endif NULL }; int main () { const char **mv; for (mv = macro_values; *mv != NULL; mv++) { const char *value = *mv; /* Test whether it looks like a cast expression. */ if (strncmp (value, "((unsigned int)"/*)*/, 15) == 0 || strncmp (value, "((unsigned short)"/*)*/, 17) == 0 || strncmp (value, "((unsigned char)"/*)*/, 16) == 0 || strncmp (value, "((int)"/*)*/, 6) == 0 || strncmp (value, "((signed short)"/*)*/, 15) == 0 || strncmp (value, "((signed char)"/*)*/, 14) == 0) return mv - macro_values + 1; } return 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_header_working_stdint_h=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_working_stdint_h" >&5 $as_echo "$gl_cv_header_working_stdint_h" >&6; } fi HAVE_C99_STDINT_H=0 HAVE_SYS_BITYPES_H=0 HAVE_SYS_INTTYPES_H=0 STDINT_H=stdint.h case "$gl_cv_header_working_stdint_h" in *yes) HAVE_C99_STDINT_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stdint.h predates C++11" >&5 $as_echo_n "checking whether stdint.h predates C++11... " >&6; } if ${gl_cv_header_stdint_predates_cxx11_h+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_header_stdint_predates_cxx11_h=yes cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #include /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif intmax_t im = INTMAX_MAX; int32_t i32 = INT32_C (0x7fffffff); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_stdint_predates_cxx11_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_stdint_predates_cxx11_h" >&5 $as_echo "$gl_cv_header_stdint_predates_cxx11_h" >&6; } if test "$gl_cv_header_stdint_predates_cxx11_h" = yes; then $as_echo "#define __STDC_CONSTANT_MACROS 1" >>confdefs.h $as_echo "#define __STDC_LIMIT_MACROS 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stdint.h has UINTMAX_WIDTH etc." >&5 $as_echo_n "checking whether stdint.h has UINTMAX_WIDTH etc.... " >&6; } if ${gl_cv_header_stdint_width+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_header_stdint_width=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif int iw = UINTMAX_WIDTH; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_stdint_width=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_stdint_width" >&5 $as_echo "$gl_cv_header_stdint_width" >&6; } if test "$gl_cv_header_stdint_width" = yes; then STDINT_H= fi ;; *) for ac_header in sys/inttypes.h sys/bitypes.h do : as_ac_Header=`$as_echo "ac_cv_header_$ac_header" | $as_tr_sh` ac_fn_c_check_header_mongrel "$LINENO" "$ac_header" "$as_ac_Header" "$ac_includes_default" if eval test \"x\$"$as_ac_Header"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done if test $ac_cv_header_sys_inttypes_h = yes; then HAVE_SYS_INTTYPES_H=1 fi if test $ac_cv_header_sys_bitypes_h = yes; then HAVE_SYS_BITYPES_H=1 fi if test $APPLE_UNIVERSAL_BUILD = 0; then for gltype in ptrdiff_t size_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking for bit size of $gltype" >&5 $as_echo_n "checking for bit size of $gltype... " >&6; } if eval \${gl_cv_bitsizeof_${gltype}+:} false; then : $as_echo_n "(cached) " >&6 else if ac_fn_c_compute_int "$LINENO" "sizeof ($gltype) * CHAR_BIT" "result" " /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif #include "; then : else result=unknown fi eval gl_cv_bitsizeof_${gltype}=\$result fi eval ac_res=\$gl_cv_bitsizeof_${gltype} { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } eval result=\$gl_cv_bitsizeof_${gltype} if test $result = unknown; then result=0 fi GLTYPE=`echo "$gltype" | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` cat >>confdefs.h <<_ACEOF #define BITSIZEOF_${GLTYPE} $result _ACEOF eval BITSIZEOF_${GLTYPE}=\$result done fi for gltype in sig_atomic_t wchar_t wint_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking for bit size of $gltype" >&5 $as_echo_n "checking for bit size of $gltype... " >&6; } if eval \${gl_cv_bitsizeof_${gltype}+:} false; then : $as_echo_n "(cached) " >&6 else if ac_fn_c_compute_int "$LINENO" "sizeof ($gltype) * CHAR_BIT" "result" " /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif #include "; then : else result=unknown fi eval gl_cv_bitsizeof_${gltype}=\$result fi eval ac_res=\$gl_cv_bitsizeof_${gltype} { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } eval result=\$gl_cv_bitsizeof_${gltype} if test $result = unknown; then result=0 fi GLTYPE=`echo "$gltype" | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` cat >>confdefs.h <<_ACEOF #define BITSIZEOF_${GLTYPE} $result _ACEOF eval BITSIZEOF_${GLTYPE}=\$result done for gltype in sig_atomic_t wchar_t wint_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gltype is signed" >&5 $as_echo_n "checking whether $gltype is signed... " >&6; } if eval \${gl_cv_type_${gltype}_signed+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif int verify[2 * (($gltype) -1 < ($gltype) 0) - 1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : result=yes else result=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext eval gl_cv_type_${gltype}_signed=\$result fi eval ac_res=\$gl_cv_type_${gltype}_signed { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } eval result=\$gl_cv_type_${gltype}_signed GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` if test "$result" = yes; then cat >>confdefs.h <<_ACEOF #define HAVE_SIGNED_${GLTYPE} 1 _ACEOF eval HAVE_SIGNED_${GLTYPE}=1 else eval HAVE_SIGNED_${GLTYPE}=0 fi done gl_cv_type_ptrdiff_t_signed=yes gl_cv_type_size_t_signed=no if test $APPLE_UNIVERSAL_BUILD = 0; then for gltype in ptrdiff_t size_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $gltype integer literal suffix" >&5 $as_echo_n "checking for $gltype integer literal suffix... " >&6; } if eval \${gl_cv_type_${gltype}_suffix+:} false; then : $as_echo_n "(cached) " >&6 else eval gl_cv_type_${gltype}_suffix=no eval result=\$gl_cv_type_${gltype}_signed if test "$result" = yes; then glsufu= else glsufu=u fi for glsuf in "$glsufu" ${glsufu}l ${glsufu}ll ${glsufu}i64; do case $glsuf in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; i64) gltype1='__int64';; u) gltype1='unsigned int';; ul) gltype1='unsigned long int';; ull) gltype1='unsigned long long int';; ui64)gltype1='unsigned __int64';; esac cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif extern $gltype foo; extern $gltype1 foo; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval gl_cv_type_${gltype}_suffix=\$glsuf fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext eval result=\$gl_cv_type_${gltype}_suffix test "$result" != no && break done fi eval ac_res=\$gl_cv_type_${gltype}_suffix { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` eval result=\$gl_cv_type_${gltype}_suffix test "$result" = no && result= eval ${GLTYPE}_SUFFIX=\$result cat >>confdefs.h <<_ACEOF #define ${GLTYPE}_SUFFIX $result _ACEOF done fi for gltype in sig_atomic_t wchar_t wint_t ; do { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $gltype integer literal suffix" >&5 $as_echo_n "checking for $gltype integer literal suffix... " >&6; } if eval \${gl_cv_type_${gltype}_suffix+:} false; then : $as_echo_n "(cached) " >&6 else eval gl_cv_type_${gltype}_suffix=no eval result=\$gl_cv_type_${gltype}_signed if test "$result" = yes; then glsufu= else glsufu=u fi for glsuf in "$glsufu" ${glsufu}l ${glsufu}ll ${glsufu}i64; do case $glsuf in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; i64) gltype1='__int64';; u) gltype1='unsigned int';; ul) gltype1='unsigned long int';; ull) gltype1='unsigned long long int';; ui64)gltype1='unsigned __int64';; esac cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif extern $gltype foo; extern $gltype1 foo; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval gl_cv_type_${gltype}_suffix=\$glsuf fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext eval result=\$gl_cv_type_${gltype}_suffix test "$result" != no && break done fi eval ac_res=\$gl_cv_type_${gltype}_suffix { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` eval result=\$gl_cv_type_${gltype}_suffix test "$result" = no && result= eval ${GLTYPE}_SUFFIX=\$result cat >>confdefs.h <<_ACEOF #define ${GLTYPE}_SUFFIX $result _ACEOF done if test $GNULIB_OVERRIDES_WINT_T = 1; then BITSIZEOF_WINT_T=32 fi ;; esac LIMITS_H=limits.h if test -n "$LIMITS_H"; then GL_GENERATE_LIMITS_H_TRUE= GL_GENERATE_LIMITS_H_FALSE='#' else GL_GENERATE_LIMITS_H_TRUE='#' GL_GENERATE_LIMITS_H_FALSE= fi if test -n "$STDINT_H"; then GL_GENERATE_STDINT_H_TRUE= GL_GENERATE_STDINT_H_FALSE='#' else GL_GENERATE_STDINT_H_TRUE='#' GL_GENERATE_STDINT_H_FALSE= fi GNULIB_IMAXABS=0; GNULIB_IMAXDIV=0; GNULIB_STRTOIMAX=0; GNULIB_STRTOUMAX=0; HAVE_DECL_IMAXABS=1; HAVE_DECL_IMAXDIV=1; HAVE_DECL_STRTOIMAX=1; HAVE_DECL_STRTOUMAX=1; REPLACE_STRTOIMAX=0; REPLACE_STRTOUMAX=0; INT32_MAX_LT_INTMAX_MAX=1; INT64_MAX_EQ_LONG_MAX='defined _LP64'; PRI_MACROS_BROKEN=0; PRIPTR_PREFIX=__PRIPTR_PREFIX; UINT32_MAX_LT_UINTMAX_MAX=1; UINT64_MAX_EQ_ULONG_MAX='defined _LP64'; if test $gl_cv_have_include_next = yes; then gl_cv_next_inttypes_h='<'inttypes.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_inttypes_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_inttypes_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'inttypes.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_inttypes_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_inttypes_h gl_cv_next_inttypes_h='"'$gl_header'"' else gl_cv_next_inttypes_h='<'inttypes.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_inttypes_h" >&5 $as_echo "$gl_cv_next_inttypes_h" >&6; } fi NEXT_INTTYPES_H=$gl_cv_next_inttypes_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'inttypes.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_inttypes_h fi NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H=$gl_next_as_first_directive for gl_func in imaxabs imaxdiv strtoimax strtoumax; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done for ac_header in inttypes.h do : ac_fn_c_check_header_mongrel "$LINENO" "inttypes.h" "ac_cv_header_inttypes_h" "$ac_includes_default" if test "x$ac_cv_header_inttypes_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_INTTYPES_H 1 _ACEOF fi done if test $ac_cv_header_inttypes_h = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether the inttypes.h PRIxNN macros are broken" >&5 $as_echo_n "checking whether the inttypes.h PRIxNN macros are broken... " >&6; } if ${gt_cv_inttypes_pri_broken+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef PRId32 char *p = PRId32; #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_inttypes_pri_broken=no else gt_cv_inttypes_pri_broken=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_inttypes_pri_broken" >&5 $as_echo "$gt_cv_inttypes_pri_broken" >&6; } fi if test "$gt_cv_inttypes_pri_broken" = yes; then cat >>confdefs.h <<_ACEOF #define PRI_MACROS_BROKEN 1 _ACEOF PRI_MACROS_BROKEN=1 else PRI_MACROS_BROKEN=0 fi GNULIB_ISWBLANK=0; GNULIB_WCTYPE=0; GNULIB_ISWCTYPE=0; GNULIB_WCTRANS=0; GNULIB_TOWCTRANS=0; HAVE_ISWBLANK=1; HAVE_WCTYPE_T=1; HAVE_WCTRANS_T=1; REPLACE_ISWBLANK=0; if test $ac_cv_header_crtdefs_h = yes; then HAVE_CRTDEFS_H=1 else HAVE_CRTDEFS_H=0 fi if test $ac_cv_func_iswcntrl = yes; then HAVE_ISWCNTRL=1 else HAVE_ISWCNTRL=0 fi if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_wctype_h='<'wctype.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_wctype_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_wctype_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'wctype.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_wctype_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_wctype_h gl_cv_next_wctype_h='"'$gl_header'"' else gl_cv_next_wctype_h='<'wctype.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_wctype_h" >&5 $as_echo "$gl_cv_next_wctype_h" >&6; } fi NEXT_WCTYPE_H=$gl_cv_next_wctype_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'wctype.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_wctype_h fi NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H=$gl_next_as_first_directive if test $ac_cv_header_wctype_h = yes; then if test $ac_cv_func_iswcntrl = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether iswcntrl works" >&5 $as_echo_n "checking whether iswcntrl works... " >&6; } if ${gl_cv_func_iswcntrl_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNU_LIBRARY__ == 1 Linux libc5 i18n is broken. #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_iswcntrl_works="guessing yes" else gl_cv_func_iswcntrl_works="guessing no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { return iswprint ('x') == 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_iswcntrl_works=yes else gl_cv_func_iswcntrl_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_iswcntrl_works" >&5 $as_echo "$gl_cv_func_iswcntrl_works" >&6; } fi HAVE_WCTYPE_H=1 else HAVE_WCTYPE_H=0 fi case "$gl_cv_func_iswcntrl_works" in *yes) REPLACE_ISWCNTRL=0 ;; *) REPLACE_ISWCNTRL=1 ;; esac if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then : fi if test $REPLACE_ISWCNTRL = 1; then REPLACE_TOWLOWER=1 else for ac_func in towlower do : ac_fn_c_check_func "$LINENO" "towlower" "ac_cv_func_towlower" if test "x$ac_cv_func_towlower" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_TOWLOWER 1 _ACEOF fi done if test $ac_cv_func_towlower = yes; then REPLACE_TOWLOWER=0 else ac_fn_c_check_decl "$LINENO" "towlower" "ac_cv_have_decl_towlower" "/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif " if test "x$ac_cv_have_decl_towlower" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_TOWLOWER $ac_have_decl _ACEOF if test $ac_cv_have_decl_towlower = yes; then REPLACE_TOWLOWER=1 else REPLACE_TOWLOWER=0 fi fi fi if test $HAVE_ISWCNTRL = 0 || test $REPLACE_TOWLOWER = 1; then : fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wctype_t" >&5 $as_echo_n "checking for wctype_t... " >&6; } if ${gl_cv_type_wctype_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif wctype_t a; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wctype_t=yes else gl_cv_type_wctype_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wctype_t" >&5 $as_echo "$gl_cv_type_wctype_t" >&6; } if test $gl_cv_type_wctype_t = no; then HAVE_WCTYPE_T=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wctrans_t" >&5 $as_echo_n "checking for wctrans_t... " >&6; } if ${gl_cv_type_wctrans_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include wctrans_t a; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wctrans_t=yes else gl_cv_type_wctrans_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wctrans_t" >&5 $as_echo "$gl_cv_type_wctrans_t" >&6; } if test $gl_cv_type_wctrans_t = no; then HAVE_WCTRANS_T=0 fi for gl_func in wctype iswctype wctrans towctrans ; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done GNULIB_NL_LANGINFO=0; HAVE_NL_LANGINFO=1; REPLACE_NL_LANGINFO=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working fcntl.h" >&5 $as_echo_n "checking for working fcntl.h... " >&6; } if ${gl_cv_header_working_fcntl_h+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess 'no' on native Windows. mingw*) gl_cv_header_working_fcntl_h='no' ;; *) gl_cv_header_working_fcntl_h=cross-compiling ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_UNISTD_H # include #else /* on Windows with MSVC */ # include # include # defined sleep(n) _sleep ((n) * 1000) #endif #include #ifndef O_NOATIME #define O_NOATIME 0 #endif #ifndef O_NOFOLLOW #define O_NOFOLLOW 0 #endif static int const constants[] = { O_CREAT, O_EXCL, O_NOCTTY, O_TRUNC, O_APPEND, O_NONBLOCK, O_SYNC, O_ACCMODE, O_RDONLY, O_RDWR, O_WRONLY }; int main () { int result = !constants; #if HAVE_SYMLINK { static char const sym[] = "conftest.sym"; if (symlink ("/dev/null", sym) != 0) result |= 2; else { int fd = open (sym, O_WRONLY | O_NOFOLLOW | O_CREAT, 0); if (fd >= 0) { close (fd); result |= 4; } } if (unlink (sym) != 0 || symlink (".", sym) != 0) result |= 2; else { int fd = open (sym, O_RDONLY | O_NOFOLLOW); if (fd >= 0) { close (fd); result |= 4; } } unlink (sym); } #endif { static char const file[] = "confdefs.h"; int fd = open (file, O_RDONLY | O_NOATIME); if (fd < 0) result |= 8; else { struct stat st0; if (fstat (fd, &st0) != 0) result |= 16; else { char c; sleep (1); if (read (fd, &c, 1) != 1) result |= 24; else { if (close (fd) != 0) result |= 32; else { struct stat st1; if (stat (file, &st1) != 0) result |= 40; else if (st0.st_atime != st1.st_atime) result |= 64; } } } } } return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_header_working_fcntl_h=yes else case $? in #( 4) gl_cv_header_working_fcntl_h='no (bad O_NOFOLLOW)';; #( 64) gl_cv_header_working_fcntl_h='no (bad O_NOATIME)';; #( 68) gl_cv_header_working_fcntl_h='no (bad O_NOATIME, O_NOFOLLOW)';; #( *) gl_cv_header_working_fcntl_h='no';; esac fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_working_fcntl_h" >&5 $as_echo "$gl_cv_header_working_fcntl_h" >&6; } case $gl_cv_header_working_fcntl_h in #( *O_NOATIME* | no | cross-compiling) ac_val=0;; #( *) ac_val=1;; esac cat >>confdefs.h <<_ACEOF #define HAVE_WORKING_O_NOATIME $ac_val _ACEOF case $gl_cv_header_working_fcntl_h in #( *O_NOFOLLOW* | no | cross-compiling) ac_val=0;; #( *) ac_val=1;; esac cat >>confdefs.h <<_ACEOF #define HAVE_WORKING_O_NOFOLLOW $ac_val _ACEOF { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether we are using the GNU C Library >= 2.1 or uClibc" >&5 $as_echo_n "checking whether we are using the GNU C Library >= 2.1 or uClibc... 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" >&6; } if ${gl_cv_have_weak+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_have_weak=no cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ extern void xyzzy (); #pragma weak xyzzy int main () { xyzzy(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_have_weak=maybe fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test $gl_cv_have_weak = maybe; then if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __ELF__ Extensible Linking Format #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Extensible Linking Format" >/dev/null 2>&1; then : gl_cv_have_weak="guessing yes" else gl_cv_have_weak="guessing no" fi rm -f conftest* else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #pragma weak fputs int main () { return (fputs == NULL); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_have_weak=yes else gl_cv_have_weak=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi case " $LDFLAGS " in *" -static "*) gl_cv_have_weak=no ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_have_weak" >&5 $as_echo "$gl_cv_have_weak" >&6; } if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # On OSF/1, the compiler needs the flag -pthread or -D_REENTRANT so that # it groks . 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then additional_libdir="$withval/$acl_libdirstem2" fi fi fi fi LIBPTH= LTLIBPTH= INCPTH= LIBPTH_PREFIX= HAVE_LIBPTH= rpathdirs= ltrpathdirs= names_already_handled= names_next_round='pth ' while test -n "$names_next_round"; do names_this_round="$names_next_round" names_next_round= for name in $names_this_round; do already_handled= for n in $names_already_handled; do if test "$n" = "$name"; then already_handled=yes break fi done if test -z "$already_handled"; then names_already_handled="$names_already_handled $name" uppername=`echo "$name" | sed -e 'y|abcdefghijklmnopqrstuvwxyz./+-|ABCDEFGHIJKLMNOPQRSTUVWXYZ____|'` eval value=\"\$HAVE_LIB$uppername\" if test -n "$value"; then if test "$value" = yes; then eval value=\"\$LIB$uppername\" test -z "$value" || LIBPTH="${LIBPTH}${LIBPTH:+ }$value" eval value=\"\$LTLIB$uppername\" test -z "$value" || LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }$value" else : fi else found_dir= found_la= found_so= found_a= eval libname=\"$acl_libname_spec\" # typically: libname=lib$name if test -n "$acl_shlibext"; then shrext=".$acl_shlibext" # typically: shrext=.so else shrext= fi if test $use_additional = yes; then dir="$additional_libdir" if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi fi if test "X$found_dir" = "X"; then for x in $LDFLAGS $LTLIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" case "$x" in -L*) dir=`echo "X$x" | sed -e 's/^X-L//'` if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi ;; esac if test "X$found_dir" != "X"; then break fi done fi if test "X$found_dir" != "X"; then LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-L$found_dir -l$name" if test "X$found_so" != "X"; then if test "$enable_rpath" = no \ || test "X$found_dir" = "X/usr/$acl_libdirstem" \ || test "X$found_dir" = "X/usr/$acl_libdirstem2"; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" else haveit= for x in $ltrpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $found_dir" fi if test "$acl_hardcode_direct" = yes; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" else if test -n "$acl_hardcode_libdir_flag_spec" && test "$acl_hardcode_minus_L" = no; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" haveit= for x in $rpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $found_dir" fi else haveit= for x in $LDFLAGS $LIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-L$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then LIBPTH="${LIBPTH}${LIBPTH:+ }-L$found_dir" fi if test "$acl_hardcode_minus_L" != no; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_so" else LIBPTH="${LIBPTH}${LIBPTH:+ }-l$name" fi fi fi fi else if test "X$found_a" != "X"; then LIBPTH="${LIBPTH}${LIBPTH:+ }$found_a" else LIBPTH="${LIBPTH}${LIBPTH:+ }-L$found_dir -l$name" fi fi additional_includedir= case "$found_dir" in */$acl_libdirstem | */$acl_libdirstem/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem/"'*$,,'` if test "$name" = 'pth'; then LIBPTH_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; */$acl_libdirstem2 | */$acl_libdirstem2/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem2/"'*$,,'` if test "$name" = 'pth'; then LIBPTH_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; esac if test "X$additional_includedir" != "X"; then if test "X$additional_includedir" != "X/usr/include"; then haveit= if test "X$additional_includedir" = "X/usr/local/include"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then for x in $CPPFLAGS $INCPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-I$additional_includedir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_includedir"; then INCPTH="${INCPTH}${INCPTH:+ }-I$additional_includedir" fi fi fi fi fi if test -n "$found_la"; then save_libdir="$libdir" case "$found_la" in */* | *\\*) . "$found_la" ;; *) . "./$found_la" ;; esac libdir="$save_libdir" for dep in $dependency_libs; do case "$dep" in -L*) additional_libdir=`echo "X$dep" | sed -e 's/^X-L//'` if test "X$additional_libdir" != "X/usr/$acl_libdirstem" \ && test "X$additional_libdir" != "X/usr/$acl_libdirstem2"; then haveit= if test "X$additional_libdir" = "X/usr/local/$acl_libdirstem" \ || test "X$additional_libdir" = "X/usr/local/$acl_libdirstem2"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then haveit= for x in $LDFLAGS $LIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then LIBPTH="${LIBPTH}${LIBPTH:+ }-L$additional_libdir" fi fi haveit= for x in $LDFLAGS $LTLIBPTH; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-L$additional_libdir" fi fi fi fi ;; -R*) dir=`echo "X$dep" | sed -e 's/^X-R//'` if test "$enable_rpath" != no; then haveit= for x in $rpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $dir" fi haveit= for x in $ltrpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $dir" fi fi ;; -l*) names_next_round="$names_next_round "`echo "X$dep" | sed -e 's/^X-l//'` ;; *.la) names_next_round="$names_next_round "`echo "X$dep" | sed -e 's,^X.*/,,' -e 's,^lib,,' -e 's,\.la$,,'` ;; *) LIBPTH="${LIBPTH}${LIBPTH:+ }$dep" LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }$dep" ;; esac done fi else LIBPTH="${LIBPTH}${LIBPTH:+ }-l$name" LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-l$name" fi fi fi done done if test "X$rpathdirs" != "X"; then if test -n "$acl_hardcode_libdir_separator"; then alldirs= for found_dir in $rpathdirs; do alldirs="${alldirs}${alldirs:+$acl_hardcode_libdir_separator}$found_dir" done acl_save_libdir="$libdir" libdir="$alldirs" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIBPTH="${LIBPTH}${LIBPTH:+ }$flag" else for found_dir in $rpathdirs; do acl_save_libdir="$libdir" libdir="$found_dir" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIBPTH="${LIBPTH}${LIBPTH:+ }$flag" done fi fi if test "X$ltrpathdirs" != "X"; then for found_dir in $ltrpathdirs; do LTLIBPTH="${LTLIBPTH}${LTLIBPTH:+ }-R$found_dir" done fi ac_cv_libpth_libs="$LIBPTH" ac_cv_libpth_ltlibs="$LTLIBPTH" ac_cv_libpth_cppflags="$INCPTH" ac_cv_libpth_prefix="$LIBPTH_PREFIX" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_libpth_libs" >&5 $as_echo "$ac_cv_libpth_libs" >&6; } LIBPTH="$ac_cv_libpth_libs" LTLIBPTH="$ac_cv_libpth_ltlibs" INCPTH="$ac_cv_libpth_cppflags" LIBPTH_PREFIX="$ac_cv_libpth_prefix" for element in $INCPTH; do haveit= for x in $CPPFLAGS; do acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" eval x=\"$x\" exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" if test "X$x" = "X$element"; then haveit=yes break fi done if test -z "$haveit"; then CPPFLAGS="${CPPFLAGS}${CPPFLAGS:+ }$element" fi done HAVE_LIBPTH=yes gl_have_pth= gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBPTH" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { pth_self(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_have_pth=yes fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gl_save_LIBS" if test -n "$gl_have_pth"; then gl_threads_api=pth LIBTHREAD="$LIBPTH" LTLIBTHREAD="$LTLIBPTH" LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" $as_echo "#define USE_PTH_THREADS 1" >>confdefs.h if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then $as_echo "#define USE_PTH_THREADS_WEAK 1" >>confdefs.h LIBTHREAD= LTLIBTHREAD= fi fi else CPPFLAGS="$gl_save_CPPFLAGS" fi fi if test -z "$gl_have_pthread"; then case "$gl_use_threads" in yes | windows | win32) # The 'win32' is for backward compatibility. if { case "$host_os" in mingw*) true;; *) false;; esac }; then gl_threads_api=windows $as_echo "#define USE_WINDOWS_THREADS 1" >>confdefs.h fi ;; esac fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for multithread API to use" >&5 $as_echo_n "checking for multithread API to use... 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HAVE_DECL_CBRTL=1; HAVE_DECL_CEILF=1; HAVE_DECL_CEILL=1; HAVE_DECL_COPYSIGNF=1; HAVE_DECL_COSL=1; HAVE_DECL_EXPL=1; HAVE_DECL_EXP2=1; HAVE_DECL_EXP2F=1; HAVE_DECL_EXP2L=1; HAVE_DECL_EXPM1L=1; HAVE_DECL_FLOORF=1; HAVE_DECL_FLOORL=1; HAVE_DECL_FREXPL=1; HAVE_DECL_LDEXPL=1; HAVE_DECL_LOGL=1; HAVE_DECL_LOG10L=1; HAVE_DECL_LOG2=1; HAVE_DECL_LOG2F=1; HAVE_DECL_LOG2L=1; HAVE_DECL_LOGB=1; HAVE_DECL_REMAINDER=1; HAVE_DECL_REMAINDERL=1; HAVE_DECL_RINTF=1; HAVE_DECL_ROUND=1; HAVE_DECL_ROUNDF=1; HAVE_DECL_ROUNDL=1; HAVE_DECL_SINL=1; HAVE_DECL_SQRTL=1; HAVE_DECL_TANL=1; HAVE_DECL_TRUNC=1; HAVE_DECL_TRUNCF=1; HAVE_DECL_TRUNCL=1; REPLACE_ACOSF=0; REPLACE_ASINF=0; REPLACE_ATANF=0; REPLACE_ATAN2F=0; REPLACE_CBRTF=0; REPLACE_CBRTL=0; REPLACE_CEIL=0; REPLACE_CEILF=0; REPLACE_CEILL=0; REPLACE_COSF=0; REPLACE_COSHF=0; REPLACE_EXPF=0; REPLACE_EXPM1=0; REPLACE_EXPM1F=0; REPLACE_EXP2=0; REPLACE_EXP2L=0; REPLACE_FABSL=0; REPLACE_FLOOR=0; REPLACE_FLOORF=0; REPLACE_FLOORL=0; REPLACE_FMA=0; REPLACE_FMAF=0; REPLACE_FMAL=0; REPLACE_FMOD=0; REPLACE_FMODF=0; REPLACE_FMODL=0; REPLACE_FREXPF=0; REPLACE_FREXP=0; REPLACE_FREXPL=0; REPLACE_HUGE_VAL=0; REPLACE_HYPOT=0; REPLACE_HYPOTF=0; REPLACE_HYPOTL=0; REPLACE_ILOGB=0; REPLACE_ILOGBF=0; REPLACE_ILOGBL=0; REPLACE_ISFINITE=0; REPLACE_ISINF=0; REPLACE_ISNAN=0; REPLACE_LDEXPL=0; REPLACE_LOG=0; REPLACE_LOGF=0; REPLACE_LOGL=0; REPLACE_LOG10=0; REPLACE_LOG10F=0; REPLACE_LOG10L=0; REPLACE_LOG1P=0; REPLACE_LOG1PF=0; REPLACE_LOG1PL=0; REPLACE_LOG2=0; REPLACE_LOG2F=0; REPLACE_LOG2L=0; REPLACE_LOGB=0; REPLACE_LOGBF=0; REPLACE_LOGBL=0; REPLACE_MODF=0; REPLACE_MODFF=0; REPLACE_MODFL=0; REPLACE_NAN=0; REPLACE_REMAINDER=0; REPLACE_REMAINDERF=0; REPLACE_REMAINDERL=0; REPLACE_ROUND=0; REPLACE_ROUNDF=0; REPLACE_ROUNDL=0; REPLACE_SIGNBIT=0; REPLACE_SIGNBIT_USING_GCC=0; REPLACE_SINF=0; REPLACE_SINHF=0; REPLACE_SQRTF=0; REPLACE_SQRTL=0; REPLACE_TANF=0; REPLACE_TANHF=0; REPLACE_TRUNC=0; REPLACE_TRUNCF=0; REPLACE_TRUNCL=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking for mbstate_t" >&5 $as_echo_n "checking for mbstate_t... " >&6; } if ${ac_cv_type_mbstate_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { mbstate_t x; return sizeof x; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_type_mbstate_t=yes else ac_cv_type_mbstate_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_type_mbstate_t" >&5 $as_echo "$ac_cv_type_mbstate_t" >&6; } if test $ac_cv_type_mbstate_t = yes; then $as_echo "#define HAVE_MBSTATE_T 1" >>confdefs.h else $as_echo "#define mbstate_t int" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 GNULIB_EXPLICIT_BZERO=0; GNULIB_FFSL=0; GNULIB_FFSLL=0; GNULIB_MEMCHR=0; GNULIB_MEMMEM=0; GNULIB_MEMPCPY=0; GNULIB_MEMRCHR=0; GNULIB_RAWMEMCHR=0; GNULIB_STPCPY=0; GNULIB_STPNCPY=0; GNULIB_STRCHRNUL=0; GNULIB_STRDUP=0; GNULIB_STRNCAT=0; GNULIB_STRNDUP=0; GNULIB_STRNLEN=0; GNULIB_STRPBRK=0; GNULIB_STRSEP=0; GNULIB_STRSTR=0; GNULIB_STRCASESTR=0; GNULIB_STRTOK_R=0; GNULIB_MBSLEN=0; GNULIB_MBSNLEN=0; GNULIB_MBSCHR=0; GNULIB_MBSRCHR=0; GNULIB_MBSSTR=0; GNULIB_MBSCASECMP=0; GNULIB_MBSNCASECMP=0; GNULIB_MBSPCASECMP=0; GNULIB_MBSCASESTR=0; GNULIB_MBSCSPN=0; GNULIB_MBSPBRK=0; GNULIB_MBSSPN=0; GNULIB_MBSSEP=0; GNULIB_MBSTOK_R=0; GNULIB_STRERROR=0; GNULIB_STRERROR_R=0; GNULIB_STRSIGNAL=0; GNULIB_STRVERSCMP=0; HAVE_MBSLEN=0; HAVE_EXPLICIT_BZERO=1; HAVE_FFSL=1; HAVE_FFSLL=1; HAVE_MEMCHR=1; HAVE_DECL_MEMMEM=1; HAVE_MEMPCPY=1; HAVE_DECL_MEMRCHR=1; HAVE_RAWMEMCHR=1; HAVE_STPCPY=1; HAVE_STPNCPY=1; HAVE_STRCHRNUL=1; HAVE_DECL_STRDUP=1; HAVE_DECL_STRNDUP=1; HAVE_DECL_STRNLEN=1; HAVE_STRPBRK=1; HAVE_STRSEP=1; HAVE_STRCASESTR=1; HAVE_DECL_STRTOK_R=1; HAVE_DECL_STRERROR_R=1; HAVE_DECL_STRSIGNAL=1; HAVE_STRVERSCMP=1; REPLACE_MEMCHR=0; REPLACE_MEMMEM=0; REPLACE_STPNCPY=0; REPLACE_STRCHRNUL=0; REPLACE_STRDUP=0; REPLACE_STRNCAT=0; REPLACE_STRNDUP=0; REPLACE_STRNLEN=0; REPLACE_STRSTR=0; REPLACE_STRCASESTR=0; REPLACE_STRTOK_R=0; REPLACE_STRERROR=0; REPLACE_STRERROR_R=0; REPLACE_STRSIGNAL=0; UNDEFINE_STRTOK_R=0; # Check for mmap(). 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" >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $gl_cv_have_include_next = yes; then gl_cv_next_strings_h='<'strings.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_strings_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_strings_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'strings.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_strings_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_strings_h gl_cv_next_strings_h='"'$gl_header'"' else gl_cv_next_strings_h='<'strings.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_strings_h" >&5 $as_echo "$gl_cv_next_strings_h" >&6; } fi NEXT_STRINGS_H=$gl_cv_next_strings_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'strings.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_strings_h fi NEXT_AS_FIRST_DIRECTIVE_STRINGS_H=$gl_next_as_first_directive if test $ac_cv_header_strings_h = yes; then HAVE_STRINGS_H=1 else HAVE_STRINGS_H=0 fi for gl_func in ffs strcasecmp strncasecmp; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Minix 3.1.8 has a bug: must be included before . */ #include #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done ac_fn_c_check_decl "$LINENO" "strndup" "ac_cv_have_decl_strndup" "$ac_includes_default" if test "x$ac_cv_have_decl_strndup" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_STRNDUP $ac_have_decl _ACEOF ac_fn_c_check_decl "$LINENO" "strnlen" "ac_cv_have_decl_strnlen" "$ac_includes_default" if test "x$ac_cv_have_decl_strnlen" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_STRNLEN $ac_have_decl _ACEOF { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether ldexp() can be used without linking with libm" >&5 $as_echo_n "checking whether ldexp() can be used without linking with libm... " >&6; } if ${gl_cv_func_ldexp_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __NO_MATH_INLINES # define __NO_MATH_INLINES 1 /* for glibc */ #endif #include double (*funcptr) (double, int) = ldexp; double x; int main () { return ldexp (x, -1) > 0; ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_ldexp_no_libm=yes else gl_cv_func_ldexp_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_ldexp_no_libm" >&5 $as_echo "$gl_cv_func_ldexp_no_libm" >&6; } ac_fn_c_check_decl "$LINENO" "strtok_r" "ac_cv_have_decl_strtok_r" "$ac_includes_default" if test "x$ac_cv_have_decl_strtok_r" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_STRTOK_R $ac_have_decl _ACEOF ac_fn_c_check_type "$LINENO" "pid_t" "ac_cv_type_pid_t" "$ac_includes_default" if test "x$ac_cv_type_pid_t" = xyes; then : else cat >>confdefs.h <<_ACEOF #define pid_t int _ACEOF fi ac_fn_c_check_type "$LINENO" "mode_t" "ac_cv_type_mode_t" "$ac_includes_default" if test "x$ac_cv_type_mode_t" = xyes; then : else cat >>confdefs.h <<_ACEOF #define mode_t int _ACEOF fi case "$host_os" in mingw*) { $as_echo "$as_me:${as_lineno-$LINENO}: checking for 64-bit off_t" >&5 $as_echo_n "checking for 64-bit off_t... " >&6; } if ${gl_cv_type_off_t_64+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int verify_off_t_size[sizeof (off_t) >= 8 ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_off_t_64=yes else gl_cv_type_off_t_64=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_off_t_64" >&5 $as_echo "$gl_cv_type_off_t_64" >&6; } if test $gl_cv_type_off_t_64 = no; then WINDOWS_64_BIT_OFF_T=1 else WINDOWS_64_BIT_OFF_T=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for 64-bit st_size" >&5 $as_echo_n "checking for 64-bit st_size... " >&6; } if ${gl_cv_member_st_size_64+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include struct stat buf; int verify_st_size_size[sizeof (buf.st_size) >= 8 ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_member_st_size_64=yes else gl_cv_member_st_size_64=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_member_st_size_64" >&5 $as_echo "$gl_cv_member_st_size_64" >&6; } if test $gl_cv_member_st_size_64 = no; then WINDOWS_64_BIT_ST_SIZE=1 else WINDOWS_64_BIT_ST_SIZE=0 fi ;; *) WINDOWS_64_BIT_OFF_T=0 WINDOWS_64_BIT_ST_SIZE=0 ;; esac $as_echo "#define _USE_STD_STAT 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_types_h='<'sys/types.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_types_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/types.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_types_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_types_h gl_cv_next_sys_types_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_types_h" >&5 $as_echo "$gl_cv_next_sys_types_h" >&6; } fi NEXT_SYS_TYPES_H=$gl_cv_next_sys_types_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/types.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_types_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H=$gl_next_as_first_directive WINDOWS_STAT_INODES=0 gl_libunistring_sed_extract_major='/^[0-9]/{s/^\([0-9]*\).*/\1/p;q;} i\ 0 q ' gl_libunistring_sed_extract_minor='/^[0-9][0-9]*[.][0-9]/{s/^[0-9]*[.]\([0-9]*\).*/\1/p;q;} i\ 0 q ' gl_libunistring_sed_extract_subminor='/^[0-9][0-9]*[.][0-9][0-9]*[.][0-9]/{s/^[0-9]*[.][0-9]*[.]\([0-9]*\).*/\1/p;q;} i\ 0 q ' if test "$HAVE_LIBUNISTRING" = yes; then LIBUNISTRING_VERSION_MAJOR=`echo "$LIBUNISTRING_VERSION" | sed -n -e "$gl_libunistring_sed_extract_major"` LIBUNISTRING_VERSION_MINOR=`echo "$LIBUNISTRING_VERSION" | sed -n -e "$gl_libunistring_sed_extract_minor"` LIBUNISTRING_VERSION_SUBMINOR=`echo "$LIBUNISTRING_VERSION" | sed -n -e "$gl_libunistring_sed_extract_subminor"` fi if test $ac_cv_header_features_h = yes; then HAVE_FEATURES_H=1 else HAVE_FEATURES_H=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for inttypes.h" >&5 $as_echo_n "checking for inttypes.h... " >&6; } if ${gl_cv_header_inttypes_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { uintmax_t i = (uintmax_t) -1; return !i; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_inttypes_h=yes else gl_cv_header_inttypes_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_inttypes_h" >&5 $as_echo "$gl_cv_header_inttypes_h" >&6; } if test $gl_cv_header_inttypes_h = yes; then cat >>confdefs.h <<_ACEOF #define HAVE_INTTYPES_H_WITH_UINTMAX 1 _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for stdint.h" >&5 $as_echo_n "checking for stdint.h... " >&6; } if ${gl_cv_header_stdint_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { uintmax_t i = (uintmax_t) -1; return !i; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_stdint_h=yes else gl_cv_header_stdint_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_stdint_h" >&5 $as_echo "$gl_cv_header_stdint_h" >&6; } if test $gl_cv_header_stdint_h = yes; then cat >>confdefs.h <<_ACEOF #define HAVE_STDINT_H_WITH_UINTMAX 1 _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for intmax_t" >&5 $as_echo_n "checking for intmax_t... " >&6; } if ${gt_cv_c_intmax_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_STDINT_H_WITH_UINTMAX #include #endif #if HAVE_INTTYPES_H_WITH_UINTMAX #include #endif int main () { intmax_t x = -1; return !x; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_c_intmax_t=yes else gt_cv_c_intmax_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_c_intmax_t" >&5 $as_echo "$gt_cv_c_intmax_t" >&6; } if test $gt_cv_c_intmax_t = yes; then $as_echo "#define HAVE_INTMAX_T 1" >>confdefs.h else test $ac_cv_type_long_long_int = yes \ && ac_type='long long' \ || ac_type='long' cat >>confdefs.h <<_ACEOF #define intmax_t $ac_type _ACEOF fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'double'" >&5 $as_echo_n "checking where to find the exponent in a 'double'... " >&6; } if ${gl_cv_cc_double_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined arm || defined __arm || defined __arm__ mixed_endianness #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "mixed_endianness" >/dev/null 2>&1; then : gl_cv_cc_double_expbit0="unknown" else : if ${ac_cv_c_bigendian+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_c_bigendian=unknown # See if we're dealing with a universal compiler. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # Check for potential -arch flags. It is not universal unless # there are at least two -arch flags with different values. ac_arch= ac_prev= for ac_word in $CC $CFLAGS $CPPFLAGS $LDFLAGS; do if test -n "$ac_prev"; then case $ac_word in i?86 | x86_64 | ppc | ppc64) if test -z "$ac_arch" || test "$ac_arch" = "$ac_word"; then ac_arch=$ac_word else ac_cv_c_bigendian=universal break fi ;; esac ac_prev= elif test "x$ac_word" = "x-arch"; then ac_prev=arch fi done fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $ac_cv_c_bigendian = unknown; then # See if sys/param.h defines the BYTE_ORDER macro. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if ! (defined BYTE_ORDER && defined BIG_ENDIAN \ && defined LITTLE_ENDIAN && BYTE_ORDER && BIG_ENDIAN \ && LITTLE_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if BYTE_ORDER != BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # See if defines _LITTLE_ENDIAN or _BIG_ENDIAN (e.g., Solaris). cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #if ! (defined _LITTLE_ENDIAN || defined _BIG_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to _BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #ifndef _BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # Compile a test program. if test "$cross_compiling" = yes; then : # Try to guess by grepping values from an object file. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ short int ascii_mm[] = { 0x4249, 0x4765, 0x6E44, 0x6961, 0x6E53, 0x7953, 0 }; short int ascii_ii[] = { 0x694C, 0x5454, 0x656C, 0x6E45, 0x6944, 0x6E61, 0 }; int use_ascii (int i) { return ascii_mm[i] + ascii_ii[i]; } short int ebcdic_ii[] = { 0x89D3, 0xE3E3, 0x8593, 0x95C5, 0x89C4, 0x9581, 0 }; short int ebcdic_mm[] = { 0xC2C9, 0xC785, 0x95C4, 0x8981, 0x95E2, 0xA8E2, 0 }; int use_ebcdic (int i) { return ebcdic_mm[i] + ebcdic_ii[i]; } extern int foo; int main () { return use_ascii (foo) == use_ebcdic (foo); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if grep BIGenDianSyS conftest.$ac_objext >/dev/null; then ac_cv_c_bigendian=yes fi if grep LiTTleEnDian conftest.$ac_objext >/dev/null ; then if test "$ac_cv_c_bigendian" = unknown; then ac_cv_c_bigendian=no else # finding both strings is unlikely to happen, but who knows? ac_cv_c_bigendian=unknown fi fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { /* Are we little or big endian? From Harbison&Steele. */ union { long int l; char c[sizeof (long int)]; } u; u.l = 1; return u.c[sizeof (long int) - 1] == 1; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_c_bigendian=no else ac_cv_c_bigendian=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi : case $ac_cv_c_bigendian in #( yes) gl_cv_cc_double_expbit0="word 0 bit 20";; #( no) gl_cv_cc_double_expbit0="word 1 bit 20" ;; #( universal) $as_echo "#define AC_APPLE_UNIVERSAL_BUILD 1" >>confdefs.h ;; #( *) gl_cv_cc_double_expbit0="unknown" ;; esac fi rm -f conftest* else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (double x) { memory_double m; size_t i; /* Clear it first, in case sizeof (double) < sizeof (memory_double). */ memset (&m, 0, sizeof (memory_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25); add_to_ored_words (0.5); add_to_ored_words (1.0); add_to_ored_words (2.0); add_to_ored_words (4.0); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_double_expbit0=`cat conftest.out` else gl_cv_cc_double_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_double_expbit0" >&5 $as_echo "$gl_cv_cc_double_expbit0" >&6; } case "$gl_cv_cc_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define DBL_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define DBL_EXPBIT0_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether snprintf returns a byte count as in C99" >&5 $as_echo_n "checking whether snprintf returns a byte count as in C99... " >&6; } if ${gl_cv_func_snprintf_retval_c99+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_retval_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_retval_c99="guessing no";; darwin*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_snprintf_retval_c99="guessing no";; openbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_retval_c99="guessing no";; aix*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_retval_c99="guessing no";; netbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on MSVC, no on mingw. mingw*) cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef _MSC_VER Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_func_snprintf_retval_c99="guessing yes" else gl_cv_func_snprintf_retval_c99="guessing no" fi rm -f conftest* ;; # If we don't know, assume the worst. *) gl_cv_func_snprintf_retval_c99="guessing no";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char buf[100]; int main () { strcpy (buf, "ABCDEF"); if (my_snprintf (buf, 3, "%d %d", 4567, 89) != 7) return 1; if (my_snprintf (buf, 0, "%d %d", 4567, 89) != 7) return 2; if (my_snprintf (NULL, 0, "%d %d", 4567, 89) != 7) return 3; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_snprintf_retval_c99=yes else gl_cv_func_snprintf_retval_c99=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_snprintf_retval_c99" >&5 $as_echo "$gl_cv_func_snprintf_retval_c99" >&6; } for ac_func in snprintf strnlen wcslen wcsnlen mbrtowc wcrtomb do : as_ac_var=`$as_echo "ac_cv_func_$ac_func" | $as_tr_sh` ac_fn_c_check_func "$LINENO" "$ac_func" "$as_ac_var" if eval test \"x\$"$as_ac_var"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done ac_fn_c_check_decl "$LINENO" "_snprintf" "ac_cv_have_decl__snprintf" "#include " if test "x$ac_cv_have_decl__snprintf" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL__SNPRINTF $ac_have_decl _ACEOF case "$gl_cv_func_snprintf_retval_c99" in *yes) $as_echo "#define HAVE_SNPRINTF_RETVAL_C99 1" >>confdefs.h ;; esac ac_fn_c_check_decl "$LINENO" "vsnprintf" "ac_cv_have_decl_vsnprintf" "$ac_includes_default" if test "x$ac_cv_have_decl_vsnprintf" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_VSNPRINTF $ac_have_decl _ACEOF GNULIB_SOCKET=0; GNULIB_CONNECT=0; GNULIB_ACCEPT=0; GNULIB_BIND=0; GNULIB_GETPEERNAME=0; GNULIB_GETSOCKNAME=0; GNULIB_GETSOCKOPT=0; GNULIB_LISTEN=0; GNULIB_RECV=0; GNULIB_SEND=0; GNULIB_RECVFROM=0; GNULIB_SENDTO=0; GNULIB_SETSOCKOPT=0; GNULIB_SHUTDOWN=0; GNULIB_ACCEPT4=0; HAVE_STRUCT_SOCKADDR_STORAGE=1; HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY=1; HAVE_SA_FAMILY_T=1; HAVE_ACCEPT4=1; if test $ac_cv_header_sys_socket_h = no; then for ac_header in ws2tcpip.h do : ac_fn_c_check_header_mongrel "$LINENO" "ws2tcpip.h" "ac_cv_header_ws2tcpip_h" "$ac_includes_default" if test "x$ac_cv_header_ws2tcpip_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_WS2TCPIP_H 1 _ACEOF fi done fi case "$host_os" in osf*) $as_echo "#define _POSIX_PII_SOCKET 1" >>confdefs.h ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether is self-contained" >&5 $as_echo_n "checking whether is self-contained... " >&6; } if ${gl_cv_header_sys_socket_h_selfcontained+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_sys_socket_h_selfcontained=yes else gl_cv_header_sys_socket_h_selfcontained=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_sys_socket_h_selfcontained" >&5 $as_echo "$gl_cv_header_sys_socket_h_selfcontained" >&6; } if test $gl_cv_header_sys_socket_h_selfcontained = yes; then for ac_func in shutdown do : ac_fn_c_check_func "$LINENO" "shutdown" "ac_cv_func_shutdown" if test "x$ac_cv_func_shutdown" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_SHUTDOWN 1 _ACEOF fi done if test $ac_cv_func_shutdown = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether defines the SHUT_* macros" >&5 $as_echo_n "checking whether defines the SHUT_* macros... " >&6; } if ${gl_cv_header_sys_socket_h_shut+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { int a[] = { SHUT_RD, SHUT_WR, SHUT_RDWR }; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_sys_socket_h_shut=yes else gl_cv_header_sys_socket_h_shut=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_sys_socket_h_shut" >&5 $as_echo "$gl_cv_header_sys_socket_h_shut" >&6; } if test $gl_cv_header_sys_socket_h_shut = no; then SYS_SOCKET_H='sys/socket.h' fi fi fi # We need to check for ws2tcpip.h now. if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_socket_h='<'sys/socket.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_socket_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_socket_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/socket.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_socket_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_socket_h gl_cv_next_sys_socket_h='"'$gl_header'"' else gl_cv_next_sys_socket_h='<'sys/socket.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_socket_h" >&5 $as_echo "$gl_cv_next_sys_socket_h" >&6; } fi NEXT_SYS_SOCKET_H=$gl_cv_next_sys_socket_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/socket.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_socket_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H=$gl_next_as_first_directive if test $ac_cv_header_sys_socket_h = yes; then HAVE_SYS_SOCKET_H=1 HAVE_WS2TCPIP_H=0 else HAVE_SYS_SOCKET_H=0 if test $ac_cv_header_ws2tcpip_h = yes; then HAVE_WS2TCPIP_H=1 else HAVE_WS2TCPIP_H=0 fi fi ac_fn_c_check_type "$LINENO" "struct sockaddr_storage" "ac_cv_type_struct_sockaddr_storage" " /* sys/types.h is not needed according to POSIX, but the sys/socket.h in i386-unknown-freebsd4.10 and powerpc-apple-darwin5.5 required it. */ #include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif " if test "x$ac_cv_type_struct_sockaddr_storage" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_SOCKADDR_STORAGE 1 _ACEOF fi ac_fn_c_check_type "$LINENO" "sa_family_t" "ac_cv_type_sa_family_t" " /* sys/types.h is not needed according to POSIX, but the sys/socket.h in i386-unknown-freebsd4.10 and powerpc-apple-darwin5.5 required it. */ #include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif " if test "x$ac_cv_type_sa_family_t" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_SA_FAMILY_T 1 _ACEOF fi if test $ac_cv_type_struct_sockaddr_storage = no; then HAVE_STRUCT_SOCKADDR_STORAGE=0 fi if test $ac_cv_type_sa_family_t = no; then HAVE_SA_FAMILY_T=0 fi if test $ac_cv_type_struct_sockaddr_storage != no; then ac_fn_c_check_member "$LINENO" "struct sockaddr_storage" "ss_family" "ac_cv_member_struct_sockaddr_storage_ss_family" "#include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif " if test "x$ac_cv_member_struct_sockaddr_storage_ss_family" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY 1 _ACEOF else HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY=0 fi fi if test $HAVE_STRUCT_SOCKADDR_STORAGE = 0 || test $HAVE_SA_FAMILY_T = 0 \ || test $HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = 0; then SYS_SOCKET_H='sys/socket.h' fi if test $ac_cv_header_sys_socket_h != yes; then for ac_header in winsock2.h do : ac_fn_c_check_header_mongrel "$LINENO" "winsock2.h" "ac_cv_header_winsock2_h" "$ac_includes_default" if test "x$ac_cv_header_winsock2_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_WINSOCK2_H 1 _ACEOF fi done fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi for gl_func in socket connect accept bind getpeername getsockname getsockopt listen recv send recvfrom sendto setsockopt shutdown accept4; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Some systems require prerequisite headers. */ #include #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done GNULIB_INET_NTOP=0; GNULIB_INET_PTON=0; HAVE_DECL_INET_NTOP=1; HAVE_DECL_INET_PTON=1; REPLACE_INET_NTOP=0; REPLACE_INET_PTON=0; GNULIB_ISBLANK=0; HAVE_ISBLANK=1; { $as_echo "$as_me:${as_lineno-$LINENO}: checking if environ is properly declared" >&5 $as_echo_n "checking if environ is properly declared... " >&6; } if ${gt_cv_var_environ_declaration+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_UNISTD_H #include #endif /* mingw, BeOS, Haiku declare environ in , not in . */ #include extern struct { int foo; } environ; int main () { environ.foo = 1; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_var_environ_declaration=no else gt_cv_var_environ_declaration=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_var_environ_declaration" >&5 $as_echo "$gt_cv_var_environ_declaration" >&6; } if test $gt_cv_var_environ_declaration = yes; then $as_echo "#define HAVE_ENVIRON_DECL 1" >>confdefs.h fi if test $gt_cv_var_environ_declaration != yes; then HAVE_DECL_ENVIRON=0 fi GNULIB_FCNTL=0; GNULIB_NONBLOCKING=0; GNULIB_OPEN=0; GNULIB_OPENAT=0; HAVE_FCNTL=1; HAVE_OPENAT=1; REPLACE_FCNTL=0; REPLACE_OPEN=0; REPLACE_OPENAT=0; GNULIB_FCHMODAT=0; GNULIB_FSTAT=0; GNULIB_FSTATAT=0; GNULIB_FUTIMENS=0; GNULIB_LCHMOD=0; GNULIB_LSTAT=0; GNULIB_MKDIRAT=0; GNULIB_MKFIFO=0; GNULIB_MKFIFOAT=0; GNULIB_MKNOD=0; GNULIB_MKNODAT=0; GNULIB_STAT=0; GNULIB_UTIMENSAT=0; GNULIB_OVERRIDES_STRUCT_STAT=0; HAVE_FCHMODAT=1; HAVE_FSTATAT=1; HAVE_FUTIMENS=1; HAVE_LCHMOD=1; HAVE_LSTAT=1; HAVE_MKDIRAT=1; HAVE_MKFIFO=1; HAVE_MKFIFOAT=1; HAVE_MKNOD=1; HAVE_MKNODAT=1; HAVE_UTIMENSAT=1; REPLACE_FSTAT=0; REPLACE_FSTATAT=0; REPLACE_FUTIMENS=0; REPLACE_LSTAT=0; REPLACE_MKDIR=0; REPLACE_MKFIFO=0; REPLACE_MKNOD=0; REPLACE_STAT=0; REPLACE_UTIMENSAT=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stat file-mode macros are broken" >&5 $as_echo_n "checking whether stat file-mode macros are broken... " >&6; } if ${ac_cv_header_stat_broken+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if defined S_ISBLK && defined S_IFDIR extern char c1[S_ISBLK (S_IFDIR) ? -1 : 1]; #endif #if defined S_ISBLK && defined S_IFCHR extern char c2[S_ISBLK (S_IFCHR) ? -1 : 1]; #endif #if defined S_ISLNK && defined S_IFREG extern char c3[S_ISLNK (S_IFREG) ? -1 : 1]; #endif #if defined S_ISSOCK && defined S_IFREG extern char c4[S_ISSOCK (S_IFREG) ? -1 : 1]; #endif _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_header_stat_broken=no else ac_cv_header_stat_broken=yes fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_header_stat_broken" >&5 $as_echo "$ac_cv_header_stat_broken" >&6; } if test $ac_cv_header_stat_broken = yes; then $as_echo "#define STAT_MACROS_BROKEN 1" >>confdefs.h fi if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_stat_h='<'sys/stat.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_stat_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_stat_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/stat.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_stat_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_stat_h gl_cv_next_sys_stat_h='"'$gl_header'"' else gl_cv_next_sys_stat_h='<'sys/stat.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_stat_h" >&5 $as_echo "$gl_cv_next_sys_stat_h" >&6; } fi NEXT_SYS_STAT_H=$gl_cv_next_sys_stat_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/stat.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_stat_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H=$gl_next_as_first_directive WINDOWS_STAT_TIMESPEC=0 ac_fn_c_check_type "$LINENO" "nlink_t" "ac_cv_type_nlink_t" "#include #include " if test "x$ac_cv_type_nlink_t" = xyes; then : else $as_echo "#define nlink_t int" >>confdefs.h fi for gl_func in fchmodat fstat fstatat futimens lchmod lstat mkdirat mkfifo mkfifoat mknod mknodat stat utimensat; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether getcwd (NULL, 0) allocates memory for result" >&5 $as_echo_n "checking whether getcwd (NULL, 0) allocates memory for result... " >&6; } if ${gl_cv_func_getcwd_null+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_getcwd_null="guessing yes";; # Guess yes on Cygwin. cygwin*) gl_cv_func_getcwd_null="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_getcwd_null="guessing no";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ # include # if HAVE_UNISTD_H # include # else /* on Windows with MSVC */ # include # endif # ifndef getcwd char *getcwd (); # endif int main () { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* mingw cwd does not start with '/', but getcwd does allocate. However, mingw fails to honor non-zero size. */ #else if (chdir ("/") != 0) return 1; else { char *f = getcwd (NULL, 0); if (! f) return 2; if (f[0] != '/') { free (f); return 3; } if (f[1] != '\0') { free (f); return 4; } free (f); return 0; } #endif ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_getcwd_null=yes else gl_cv_func_getcwd_null=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getcwd_null" >&5 $as_echo "$gl_cv_func_getcwd_null" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for getcwd with POSIX signature" >&5 $as_echo_n "checking for getcwd with POSIX signature... " >&6; } if ${gl_cv_func_getcwd_posix_signature+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { extern #ifdef __cplusplus "C" #endif char *getcwd (char *, size_t); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_getcwd_posix_signature=yes else gl_cv_func_getcwd_posix_signature=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_getcwd_posix_signature" >&5 $as_echo "$gl_cv_func_getcwd_posix_signature" >&6; } ac_fn_c_check_decl "$LINENO" "getdtablesize" "ac_cv_have_decl_getdtablesize" "$ac_includes_default" if test "x$ac_cv_have_decl_getdtablesize" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_GETDTABLESIZE $ac_have_decl _ACEOF GNULIB_GETTIMEOFDAY=0; HAVE_GETTIMEOFDAY=1; HAVE_STRUCT_TIMEVAL=1; HAVE_SYS_TIME_H=1; REPLACE_GETTIMEOFDAY=0; REPLACE_STRUCT_TIMEVAL=0; if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_time_h='<'sys/time.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_time_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_time_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/time.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_time_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_time_h gl_cv_next_sys_time_h='"'$gl_header'"' else gl_cv_next_sys_time_h='<'sys/time.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_time_h" >&5 $as_echo "$gl_cv_next_sys_time_h" >&6; } fi NEXT_SYS_TIME_H=$gl_cv_next_sys_time_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/time.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_time_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H=$gl_next_as_first_directive if test $ac_cv_header_sys_time_h != yes; then HAVE_SYS_TIME_H=0 fi if test $ac_cv_header_sys_socket_h != yes; then for ac_header in winsock2.h do : ac_fn_c_check_header_mongrel "$LINENO" "winsock2.h" "ac_cv_header_winsock2_h" "$ac_includes_default" if test "x$ac_cv_header_winsock2_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_WINSOCK2_H 1 _ACEOF fi done fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timeval" >&5 $as_echo_n "checking for struct timeval... " >&6; } if ${gl_cv_sys_struct_timeval+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif int main () { static struct timeval x; x.tv_sec = x.tv_usec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timeval=yes else gl_cv_sys_struct_timeval=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timeval" >&5 $as_echo "$gl_cv_sys_struct_timeval" >&6; } if test $gl_cv_sys_struct_timeval != yes; then HAVE_STRUCT_TIMEVAL=0 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wide-enough struct timeval.tv_sec member" >&5 $as_echo_n "checking for wide-enough struct timeval.tv_sec member... " >&6; } if ${gl_cv_sys_struct_timeval_tv_sec+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif int main () { static struct timeval x; typedef int verify_tv_sec_type[ sizeof (time_t) <= sizeof x.tv_sec ? 1 : -1 ]; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timeval_tv_sec=yes else gl_cv_sys_struct_timeval_tv_sec=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timeval_tv_sec" >&5 $as_echo "$gl_cv_sys_struct_timeval_tv_sec" >&6; } if test $gl_cv_sys_struct_timeval_tv_sec != yes; then REPLACE_STRUCT_TIMEVAL=1 fi fi for gl_func in gettimeofday; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_SYS_TIME_H # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done NEED_LOCALTIME_BUFFER=0 GNULIB_CTIME=0; GNULIB_MKTIME=0; GNULIB_LOCALTIME=0; GNULIB_NANOSLEEP=0; GNULIB_STRFTIME=0; GNULIB_STRPTIME=0; GNULIB_TIMEGM=0; GNULIB_TIME_R=0; GNULIB_TIME_RZ=0; GNULIB_TZSET=0; HAVE_DECL_LOCALTIME_R=1; HAVE_NANOSLEEP=1; HAVE_STRPTIME=1; HAVE_TIMEGM=1; HAVE_TZSET=1; HAVE_TIMEZONE_T=0; REPLACE_CTIME=GNULIB_PORTCHECK; REPLACE_LOCALTIME_R=GNULIB_PORTCHECK; REPLACE_MKTIME=GNULIB_PORTCHECK; REPLACE_NANOSLEEP=GNULIB_PORTCHECK; REPLACE_STRFTIME=GNULIB_PORTCHECK; REPLACE_TIMEGM=GNULIB_PORTCHECK; REPLACE_TZSET=GNULIB_PORTCHECK; : ${GNULIB_GETTIMEOFDAY=0}; REPLACE_GMTIME=0; REPLACE_LOCALTIME=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking for IPv4 sockets" >&5 $as_echo_n "checking for IPv4 sockets... " >&6; } if ${gl_cv_socket_ipv4+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_NETINET_IN_H #include #endif #ifdef HAVE_WINSOCK2_H #include #endif int main () { int x = AF_INET; struct in_addr y; struct sockaddr_in z; if (&x && &y && &z) return 0; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_socket_ipv4=yes else gl_cv_socket_ipv4=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_socket_ipv4" >&5 $as_echo "$gl_cv_socket_ipv4" >&6; } if test $gl_cv_socket_ipv4 = yes; then $as_echo "#define HAVE_IPV4 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for IPv6 sockets" >&5 $as_echo_n "checking for IPv6 sockets... " >&6; } if ${gl_cv_socket_ipv6+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_NETINET_IN_H #include #endif #ifdef HAVE_WINSOCK2_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif int main () { int x = AF_INET6; struct in6_addr y; struct sockaddr_in6 z; if (&x && &y && &z) return 0; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_socket_ipv6=yes else gl_cv_socket_ipv6=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_socket_ipv6" >&5 $as_echo "$gl_cv_socket_ipv6" >&6; } if test $gl_cv_socket_ipv6 = yes; then $as_echo "#define HAVE_IPV6 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'float'" >&5 $as_echo_n "checking where to find the exponent in a 'float'... " >&6; } if ${gl_cv_cc_float_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_float_expbit0="word 0 bit 23" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (float x) { memory_float m; size_t i; /* Clear it first, in case sizeof (float) < sizeof (memory_float). */ memset (&m, 0, sizeof (memory_float)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25f); add_to_ored_words (0.5f); add_to_ored_words (1.0f); add_to_ored_words (2.0f); add_to_ored_words (4.0f); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_float_expbit0=`cat conftest.out` else gl_cv_cc_float_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_float_expbit0" >&5 $as_echo "$gl_cv_cc_float_expbit0" >&6; } case "$gl_cv_cc_float_expbit0" in word*bit*) word=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define FLT_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define FLT_EXPBIT0_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether byte ordering is bigendian" >&5 $as_echo_n "checking whether byte ordering is bigendian... " >&6; } if ${ac_cv_c_bigendian+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_c_bigendian=unknown # See if we're dealing with a universal compiler. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # Check for potential -arch flags. It is not universal unless # there are at least two -arch flags with different values. ac_arch= ac_prev= for ac_word in $CC $CFLAGS $CPPFLAGS $LDFLAGS; do if test -n "$ac_prev"; then case $ac_word in i?86 | x86_64 | ppc | ppc64) if test -z "$ac_arch" || test "$ac_arch" = "$ac_word"; then ac_arch=$ac_word else ac_cv_c_bigendian=universal break fi ;; esac ac_prev= elif test "x$ac_word" = "x-arch"; then ac_prev=arch fi done fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $ac_cv_c_bigendian = unknown; then # See if sys/param.h defines the BYTE_ORDER macro. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if ! (defined BYTE_ORDER && defined BIG_ENDIAN \ && defined LITTLE_ENDIAN && BYTE_ORDER && BIG_ENDIAN \ && LITTLE_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if BYTE_ORDER != BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # See if defines _LITTLE_ENDIAN or _BIG_ENDIAN (e.g., Solaris). cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #if ! (defined _LITTLE_ENDIAN || defined _BIG_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to _BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #ifndef _BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # Compile a test program. if test "$cross_compiling" = yes; then : # Try to guess by grepping values from an object file. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ short int ascii_mm[] = { 0x4249, 0x4765, 0x6E44, 0x6961, 0x6E53, 0x7953, 0 }; short int ascii_ii[] = { 0x694C, 0x5454, 0x656C, 0x6E45, 0x6944, 0x6E61, 0 }; int use_ascii (int i) { return ascii_mm[i] + ascii_ii[i]; } short int ebcdic_ii[] = { 0x89D3, 0xE3E3, 0x8593, 0x95C5, 0x89C4, 0x9581, 0 }; short int ebcdic_mm[] = { 0xC2C9, 0xC785, 0x95C4, 0x8981, 0x95E2, 0xA8E2, 0 }; int use_ebcdic (int i) { return ebcdic_mm[i] + ebcdic_ii[i]; } extern int foo; int main () { return use_ascii (foo) == use_ebcdic (foo); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if grep BIGenDianSyS conftest.$ac_objext >/dev/null; then ac_cv_c_bigendian=yes fi if grep LiTTleEnDian conftest.$ac_objext >/dev/null ; then if test "$ac_cv_c_bigendian" = unknown; then ac_cv_c_bigendian=no else # finding both strings is unlikely to happen, but who knows? ac_cv_c_bigendian=unknown fi fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { /* Are we little or big endian? From Harbison&Steele. */ union { long int l; char c[sizeof (long int)]; } u; u.l = 1; return u.c[sizeof (long int) - 1] == 1; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_c_bigendian=no else ac_cv_c_bigendian=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_c_bigendian" >&5 $as_echo "$ac_cv_c_bigendian" >&6; } case $ac_cv_c_bigendian in #( yes) $as_echo "#define WORDS_BIGENDIAN 1" >>confdefs.h ;; #( no) ;; #( universal) $as_echo "#define AC_APPLE_UNIVERSAL_BUILD 1" >>confdefs.h ;; #( *) as_fn_error $? "unknown endianness presetting ac_cv_c_bigendian=no (or yes) will help" "$LINENO" 5 ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether long double and double are the same" >&5 $as_echo_n "checking whether long double and double are the same... " >&6; } if ${gl_cv_long_double_equals_double+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { typedef int check[sizeof (long double) == sizeof (double) && LDBL_MANT_DIG == DBL_MANT_DIG && LDBL_MAX_EXP == DBL_MAX_EXP && LDBL_MIN_EXP == DBL_MIN_EXP ? 1 : -1]; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_long_double_equals_double=yes else gl_cv_long_double_equals_double=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_long_double_equals_double" >&5 $as_echo "$gl_cv_long_double_equals_double" >&6; } if test $gl_cv_long_double_equals_double = yes; then $as_echo "#define HAVE_SAME_LONG_DOUBLE_AS_DOUBLE 1" >>confdefs.h HAVE_SAME_LONG_DOUBLE_AS_DOUBLE=1 else HAVE_SAME_LONG_DOUBLE_AS_DOUBLE=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for LC_MESSAGES" >&5 $as_echo_n "checking for LC_MESSAGES... " >&6; } if ${gt_cv_val_LC_MESSAGES+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { return LC_MESSAGES ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gt_cv_val_LC_MESSAGES=yes else gt_cv_val_LC_MESSAGES=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_val_LC_MESSAGES" >&5 $as_echo "$gt_cv_val_LC_MESSAGES" >&6; } if test $gt_cv_val_LC_MESSAGES = yes; then $as_echo "#define HAVE_LC_MESSAGES 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for CFPreferencesCopyAppValue" >&5 $as_echo_n "checking for CFPreferencesCopyAppValue... " >&6; } if ${gt_cv_func_CFPreferencesCopyAppValue+:} false; then : $as_echo_n "(cached) " >&6 else gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { CFPreferencesCopyAppValue(NULL, NULL) ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gt_cv_func_CFPreferencesCopyAppValue=yes else gt_cv_func_CFPreferencesCopyAppValue=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gt_save_LIBS" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_func_CFPreferencesCopyAppValue" >&5 $as_echo "$gt_cv_func_CFPreferencesCopyAppValue" >&6; } if test $gt_cv_func_CFPreferencesCopyAppValue = yes; then $as_echo "#define HAVE_CFPREFERENCESCOPYAPPVALUE 1" >>confdefs.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for CFLocaleCopyCurrent" >&5 $as_echo_n "checking for CFLocaleCopyCurrent... " >&6; } if ${gt_cv_func_CFLocaleCopyCurrent+:} false; then : $as_echo_n "(cached) " >&6 else gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { CFLocaleCopyCurrent(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gt_cv_func_CFLocaleCopyCurrent=yes else gt_cv_func_CFLocaleCopyCurrent=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gt_save_LIBS" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_func_CFLocaleCopyCurrent" >&5 $as_echo "$gt_cv_func_CFLocaleCopyCurrent" >&6; } if test $gt_cv_func_CFLocaleCopyCurrent = yes; then $as_echo "#define HAVE_CFLOCALECOPYCURRENT 1" >>confdefs.h fi INTL_MACOSX_LIBS= if test $gt_cv_func_CFPreferencesCopyAppValue = yes || test $gt_cv_func_CFLocaleCopyCurrent = yes; then INTL_MACOSX_LIBS="-Wl,-framework -Wl,CoreFoundation" fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether lstat correctly handles trailing slash" >&5 $as_echo_n "checking whether lstat correctly handles trailing slash... " >&6; } if ${gl_cv_func_lstat_dereferences_slashed_symlink+:} false; then : $as_echo_n "(cached) " >&6 else rm -f conftest.sym conftest.file echo >conftest.file if test "$cross_compiling" = yes; then : case "$host_os" in *-gnu*) # Guess yes on glibc systems. gl_cv_func_lstat_dereferences_slashed_symlink="guessing yes" ;; mingw*) # Guess no on native Windows. gl_cv_func_lstat_dereferences_slashed_symlink="guessing no" ;; *) # If we don't know, assume the worst. gl_cv_func_lstat_dereferences_slashed_symlink="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { struct stat sbuf; if (symlink ("conftest.file", "conftest.sym") != 0) return 1; /* Linux will dereference the symlink and fail, as required by POSIX. That is better in the sense that it means we will not have to compile and use the lstat wrapper. */ return lstat ("conftest.sym/", &sbuf) == 0; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_lstat_dereferences_slashed_symlink=yes else gl_cv_func_lstat_dereferences_slashed_symlink=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.sym conftest.file fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_lstat_dereferences_slashed_symlink" >&5 $as_echo "$gl_cv_func_lstat_dereferences_slashed_symlink" >&6; } case "$gl_cv_func_lstat_dereferences_slashed_symlink" in *yes) cat >>confdefs.h <<_ACEOF #define LSTAT_FOLLOWS_SLASHED_SYMLINK 1 _ACEOF ;; esac GNULIB_PSELECT=0; GNULIB_SELECT=0; HAVE_PSELECT=1; REPLACE_PSELECT=0; REPLACE_SELECT=0; { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether is self-contained" >&5 $as_echo_n "checking whether is self-contained... " >&6; } if ${gl_cv_header_sys_select_h_selfcontained+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { struct timeval b; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_sys_select_h_selfcontained=yes else gl_cv_header_sys_select_h_selfcontained=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $gl_cv_header_sys_select_h_selfcontained = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { int memset; int bzero; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef memset #define memset nonexistent_memset extern #ifdef __cplusplus "C" #endif void *memset (void *, int, unsigned long); #undef bzero #define bzero nonexistent_bzero extern #ifdef __cplusplus "C" #endif void bzero (void *, unsigned long); fd_set fds; FD_ZERO (&fds); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : else gl_cv_header_sys_select_h_selfcontained=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_sys_select_h_selfcontained" >&5 $as_echo "$gl_cv_header_sys_select_h_selfcontained" >&6; } if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_select_h='<'sys/select.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_select_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_select_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/select.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_select_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_select_h gl_cv_next_sys_select_h='"'$gl_header'"' else gl_cv_next_sys_select_h='<'sys/select.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_select_h" >&5 $as_echo "$gl_cv_next_sys_select_h" >&6; } fi NEXT_SYS_SELECT_H=$gl_cv_next_sys_select_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/select.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_select_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H=$gl_next_as_first_directive if test $ac_cv_header_sys_select_h = yes; then HAVE_SYS_SELECT_H=1 else HAVE_SYS_SELECT_H=0 fi if test $ac_cv_header_sys_socket_h != yes; then for ac_header in winsock2.h do : ac_fn_c_check_header_mongrel "$LINENO" "winsock2.h" "ac_cv_header_winsock2_h" "$ac_includes_default" if test "x$ac_cv_header_winsock2_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_WINSOCK2_H 1 _ACEOF fi done fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi for gl_func in pselect select; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Some systems require prerequisite headers. */ #include #if !(defined __GLIBC__ && !defined __UCLIBC__) && HAVE_SYS_TIME_H # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $ac_cv_header_sys_socket_h != yes; then for ac_header in winsock2.h do : ac_fn_c_check_header_mongrel "$LINENO" "winsock2.h" "ac_cv_header_winsock2_h" "$ac_includes_default" if test "x$ac_cv_header_winsock2_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_WINSOCK2_H 1 _ACEOF fi done fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi LIBSOCKET= if test $HAVE_WINSOCK2_H = 1; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking if we need to call WSAStartup in winsock2.h and -lws2_32" >&5 $as_echo_n "checking if we need to call WSAStartup in winsock2.h and -lws2_32... " >&6; } if ${gl_cv_func_wsastartup+:} false; then : $as_echo_n "(cached) " >&6 else gl_save_LIBS="$LIBS" LIBS="$LIBS -lws2_32" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef HAVE_WINSOCK2_H # include #endif int main () { WORD wVersionRequested = MAKEWORD(1, 1); WSADATA wsaData; int err = WSAStartup(wVersionRequested, &wsaData); WSACleanup (); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_wsastartup=yes else gl_cv_func_wsastartup=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext LIBS="$gl_save_LIBS" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wsastartup" >&5 $as_echo "$gl_cv_func_wsastartup" >&6; } if test "$gl_cv_func_wsastartup" = "yes"; then $as_echo "#define WINDOWS_SOCKETS 1" >>confdefs.h LIBSOCKET='-lws2_32' fi else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for library containing setsockopt" >&5 $as_echo_n "checking for library containing setsockopt... " >&6; } if ${gl_cv_lib_socket+:} false; then : $as_echo_n "(cached) " >&6 else gl_cv_lib_socket= cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ extern #ifdef __cplusplus "C" #endif char setsockopt(); int main () { setsockopt(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : else gl_save_LIBS="$LIBS" LIBS="$gl_save_LIBS -lsocket" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ extern #ifdef __cplusplus "C" #endif char setsockopt(); int main () { setsockopt(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_lib_socket="-lsocket" fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$gl_cv_lib_socket"; then LIBS="$gl_save_LIBS -lnetwork" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ extern #ifdef __cplusplus "C" #endif char setsockopt(); int main () { setsockopt(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_lib_socket="-lnetwork" fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$gl_cv_lib_socket"; then LIBS="$gl_save_LIBS -lnet" cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ extern #ifdef __cplusplus "C" #endif char setsockopt(); int main () { setsockopt(); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_lib_socket="-lnet" fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi fi LIBS="$gl_save_LIBS" fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext if test -z "$gl_cv_lib_socket"; then gl_cv_lib_socket="none needed" fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_lib_socket" >&5 $as_echo "$gl_cv_lib_socket" >&6; } if test "$gl_cv_lib_socket" != "none needed"; then LIBSOCKET="$gl_cv_lib_socket" fi fi : if test "$ac_cv_header_winsock2_h" = yes; then REPLACE_SELECT=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether select supports a 0 argument" >&5 $as_echo_n "checking whether select supports a 0 argument... " >&6; } if ${gl_cv_func_select_supports0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess no on Interix. interix*) gl_cv_func_select_supports0="guessing no";; # Guess yes otherwise. *) gl_cv_func_select_supports0="guessing yes";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_SYS_SELECT_H #include #endif int main () { struct timeval timeout; timeout.tv_sec = 0; timeout.tv_usec = 5; return select (0, (fd_set *)0, (fd_set *)0, (fd_set *)0, &timeout) < 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_select_supports0=yes else gl_cv_func_select_supports0=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_select_supports0" >&5 $as_echo "$gl_cv_func_select_supports0" >&6; } case "$gl_cv_func_select_supports0" in *yes) ;; *) REPLACE_SELECT=1 ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether select detects invalid fds" >&5 $as_echo_n "checking whether select detects invalid fds... " >&6; } if ${gl_cv_func_select_detects_ebadf+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_select_detects_ebadf="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_select_detects_ebadf="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_SYS_SELECT_H # include #endif #include #include int main () { fd_set set; dup2(0, 16); FD_ZERO(&set); FD_SET(16, &set); close(16); struct timeval timeout; timeout.tv_sec = 0; timeout.tv_usec = 5; return select (17, &set, NULL, NULL, &timeout) != -1 || errno != EBADF; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_select_detects_ebadf=yes else gl_cv_func_select_detects_ebadf=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_select_detects_ebadf" >&5 $as_echo "$gl_cv_func_select_detects_ebadf" >&6; } case $gl_cv_func_select_detects_ebadf in *yes) ;; *) REPLACE_SELECT=1 ;; esac fi LIB_SELECT="$LIBSOCKET" if test $REPLACE_SELECT = 1; then case "$host_os" in mingw*) cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #define WIN32_LEAN_AND_MEAN #include int main () { MsgWaitForMultipleObjects (0, NULL, 0, 0, 0); return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : else LIB_SELECT="$LIB_SELECT -luser32" fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for O_CLOEXEC" >&5 $as_echo_n "checking for O_CLOEXEC... " >&6; } if ${gl_cv_macro_O_CLOEXEC+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifndef O_CLOEXEC choke me; #endif int main () { return O_CLOEXEC; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_macro_O_CLOEXEC=yes else gl_cv_macro_O_CLOEXEC=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_macro_O_CLOEXEC" >&5 $as_echo "$gl_cv_macro_O_CLOEXEC" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for promoted mode_t type" >&5 $as_echo_n "checking for promoted mode_t type... 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" >&6; } if ${gl_cv_sys_struct_timespec_in_time_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { static struct timespec x; x.tv_sec = x.tv_nsec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timespec_in_time_h=yes else gl_cv_sys_struct_timespec_in_time_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timespec_in_time_h" >&5 $as_echo "$gl_cv_sys_struct_timespec_in_time_h" >&6; } TIME_H_DEFINES_STRUCT_TIMESPEC=0 SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=0 PTHREAD_H_DEFINES_STRUCT_TIMESPEC=0 UNISTD_H_DEFINES_STRUCT_TIMESPEC=0 if test $gl_cv_sys_struct_timespec_in_time_h = yes; then TIME_H_DEFINES_STRUCT_TIMESPEC=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timespec in " >&5 $as_echo_n "checking for struct timespec in ... 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" >&6; } if ${gl_cv_sys_struct_timespec_in_pthread_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { static struct timespec x; x.tv_sec = x.tv_nsec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timespec_in_pthread_h=yes else gl_cv_sys_struct_timespec_in_pthread_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timespec_in_pthread_h" >&5 $as_echo "$gl_cv_sys_struct_timespec_in_pthread_h" >&6; } if test $gl_cv_sys_struct_timespec_in_pthread_h = yes; then PTHREAD_H_DEFINES_STRUCT_TIMESPEC=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for struct timespec in " >&5 $as_echo_n "checking for struct timespec in ... " >&6; } if ${gl_cv_sys_struct_timespec_in_unistd_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { static struct timespec x; x.tv_sec = x.tv_nsec; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_timespec_in_unistd_h=yes else gl_cv_sys_struct_timespec_in_unistd_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_timespec_in_unistd_h" >&5 $as_echo "$gl_cv_sys_struct_timespec_in_unistd_h" >&6; } if test $gl_cv_sys_struct_timespec_in_unistd_h = yes; then UNISTD_H_DEFINES_STRUCT_TIMESPEC=1 fi fi fi fi if test $gl_cv_have_include_next = yes; then gl_cv_next_time_h='<'time.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... 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It is improbable that only one of them will # be defined and other not, I prefer to stay on the safe side and to # test each one separately. { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether program_invocation_name is defined" >&5 $as_echo_n "checking whether program_invocation_name is defined... " >&6; } cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { program_invocation_name = "test"; ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : $as_echo "#define HAVE_PROGRAM_INVOCATION_NAME 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: result: yes" >&5 $as_echo "yes" >&6; } else { $as_echo "$as_me:${as_lineno-$LINENO}: result: no" >&5 $as_echo "no" >&6; } fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether program_invocation_short_name is defined" >&5 $as_echo_n "checking whether program_invocation_short_name is defined... 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" >&6; } if ${gl_cv_test_INT64_MAX_EQ_LONG_MAX+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Work also in C++ mode. */ #define __STDC_LIMIT_MACROS 1 /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H #include #if HAVE_STDINT_H #include #endif #if defined INT64_MAX #define CONDITION (INT64_MAX == LONG_MAX) #elif HAVE_LONG_LONG_INT #define CONDITION (sizeof (long long int) == sizeof (long int)) #else #define CONDITION 0 #endif int test[CONDITION ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_test_INT64_MAX_EQ_LONG_MAX=yes else gl_cv_test_INT64_MAX_EQ_LONG_MAX=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_test_INT64_MAX_EQ_LONG_MAX" >&5 $as_echo "$gl_cv_test_INT64_MAX_EQ_LONG_MAX" >&6; } if test $gl_cv_test_INT64_MAX_EQ_LONG_MAX = yes; then INT64_MAX_EQ_LONG_MAX=1; else INT64_MAX_EQ_LONG_MAX=0; fi else INT64_MAX_EQ_LONG_MAX=-1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether UINT32_MAX < UINTMAX_MAX" >&5 $as_echo_n "checking whether UINT32_MAX < UINTMAX_MAX... " >&6; } if ${gl_cv_test_UINT32_MAX_LT_UINTMAX_MAX+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Work also in C++ mode. */ #define __STDC_LIMIT_MACROS 1 /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H #include #if HAVE_STDINT_H #include #endif #if defined UINT32_MAX && defined UINTMAX_MAX #define CONDITION (UINT32_MAX < UINTMAX_MAX) #elif HAVE_LONG_LONG_INT #define CONDITION (sizeof (unsigned int) < sizeof (unsigned long long int)) #else #define CONDITION 0 #endif int test[CONDITION ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_test_UINT32_MAX_LT_UINTMAX_MAX=yes else gl_cv_test_UINT32_MAX_LT_UINTMAX_MAX=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_test_UINT32_MAX_LT_UINTMAX_MAX" >&5 $as_echo "$gl_cv_test_UINT32_MAX_LT_UINTMAX_MAX" >&6; } if test $gl_cv_test_UINT32_MAX_LT_UINTMAX_MAX = yes; then UINT32_MAX_LT_UINTMAX_MAX=1; else UINT32_MAX_LT_UINTMAX_MAX=0; fi if test $APPLE_UNIVERSAL_BUILD = 0; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether UINT64_MAX == ULONG_MAX" >&5 $as_echo_n "checking whether UINT64_MAX == ULONG_MAX... " >&6; } if ${gl_cv_test_UINT64_MAX_EQ_ULONG_MAX+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Work also in C++ mode. */ #define __STDC_LIMIT_MACROS 1 /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H #include #if HAVE_STDINT_H #include #endif #if defined UINT64_MAX #define CONDITION (UINT64_MAX == ULONG_MAX) #elif HAVE_LONG_LONG_INT #define CONDITION (sizeof (unsigned long long int) == sizeof (unsigned long int)) #else #define CONDITION 0 #endif int test[CONDITION ? 1 : -1]; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_test_UINT64_MAX_EQ_ULONG_MAX=yes else gl_cv_test_UINT64_MAX_EQ_ULONG_MAX=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_test_UINT64_MAX_EQ_ULONG_MAX" >&5 $as_echo "$gl_cv_test_UINT64_MAX_EQ_ULONG_MAX" >&6; } if test $gl_cv_test_UINT64_MAX_EQ_ULONG_MAX = yes; then UINT64_MAX_EQ_ULONG_MAX=1; else UINT64_MAX_EQ_ULONG_MAX=0; fi else UINT64_MAX_EQ_ULONG_MAX=-1 fi ac_fn_c_check_decl "$LINENO" "iswblank" "ac_cv_have_decl_iswblank" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include " if test "x$ac_cv_have_decl_iswblank" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_ISWBLANK $ac_have_decl _ACEOF if test $ac_cv_func_iswblank = no; then HAVE_ISWBLANK=0 if test $ac_cv_have_decl_iswblank = yes; then REPLACE_ISWBLANK=1 fi fi if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then : else if test $HAVE_ISWBLANK = 0 || test $REPLACE_ISWBLANK = 1; then : fi fi if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then : else if test $HAVE_ISWBLANK = 0 || test $REPLACE_ISWBLANK = 1; then gl_LIBOBJS="$gl_LIBOBJS iswblank.$ac_objext" fi fi GNULIB_ISWBLANK=1 $as_echo "#define GNULIB_TEST_ISWBLANK 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_langinfo_h='<'langinfo.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_langinfo_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_langinfo_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'langinfo.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_langinfo_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_langinfo_h gl_cv_next_langinfo_h='"'$gl_header'"' else gl_cv_next_langinfo_h='<'langinfo.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_langinfo_h" >&5 $as_echo "$gl_cv_next_langinfo_h" >&6; } fi NEXT_LANGINFO_H=$gl_cv_next_langinfo_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'langinfo.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_langinfo_h fi NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H=$gl_next_as_first_directive HAVE_LANGINFO_CODESET=0 HAVE_LANGINFO_T_FMT_AMPM=0 HAVE_LANGINFO_ERA=0 HAVE_LANGINFO_YESEXPR=0 if test $ac_cv_header_langinfo_h = yes; then HAVE_LANGINFO_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines CODESET" >&5 $as_echo_n "checking whether langinfo.h defines CODESET... " >&6; } if ${gl_cv_header_langinfo_codeset+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = CODESET; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_codeset=yes else gl_cv_header_langinfo_codeset=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_codeset" >&5 $as_echo "$gl_cv_header_langinfo_codeset" >&6; } if test $gl_cv_header_langinfo_codeset = yes; then HAVE_LANGINFO_CODESET=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines T_FMT_AMPM" >&5 $as_echo_n "checking whether langinfo.h defines T_FMT_AMPM... " >&6; } if ${gl_cv_header_langinfo_t_fmt_ampm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = T_FMT_AMPM; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_t_fmt_ampm=yes else gl_cv_header_langinfo_t_fmt_ampm=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_t_fmt_ampm" >&5 $as_echo "$gl_cv_header_langinfo_t_fmt_ampm" >&6; } if test $gl_cv_header_langinfo_t_fmt_ampm = yes; then HAVE_LANGINFO_T_FMT_AMPM=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines ERA" >&5 $as_echo_n "checking whether langinfo.h defines ERA... " >&6; } if ${gl_cv_header_langinfo_era+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = ERA; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_era=yes else gl_cv_header_langinfo_era=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_era" >&5 $as_echo "$gl_cv_header_langinfo_era" >&6; } if test $gl_cv_header_langinfo_era = yes; then HAVE_LANGINFO_ERA=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether langinfo.h defines YESEXPR" >&5 $as_echo_n "checking whether langinfo.h defines YESEXPR... " >&6; } if ${gl_cv_header_langinfo_yesexpr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int a = YESEXPR; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_langinfo_yesexpr=yes else gl_cv_header_langinfo_yesexpr=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_langinfo_yesexpr" >&5 $as_echo "$gl_cv_header_langinfo_yesexpr" >&6; } if test $gl_cv_header_langinfo_yesexpr = yes; then HAVE_LANGINFO_YESEXPR=1 fi else HAVE_LANGINFO_H=0 fi for gl_func in nl_langinfo; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done LOCALCHARSET_TESTS_ENVIRONMENT="CHARSETALIASDIR=\"\$(abs_top_builddir)/$gl_source_base\"" case "$host_os" in solaris*) $as_echo "#define _LCONV_C99 1" >>confdefs.h ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether locale.h conforms to POSIX:2001" >&5 $as_echo_n "checking whether locale.h conforms to POSIX:2001... " >&6; } if ${gl_cv_header_locale_h_posix2001+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int x = LC_MESSAGES; int y = sizeof (((struct lconv *) 0)->decimal_point); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_locale_h_posix2001=yes else gl_cv_header_locale_h_posix2001=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_locale_h_posix2001" >&5 $as_echo "$gl_cv_header_locale_h_posix2001" >&6; } if test $ac_cv_header_xlocale_h = yes; then HAVE_XLOCALE_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether locale.h defines locale_t" >&5 $as_echo_n "checking whether locale.h defines locale_t... " >&6; } if ${gl_cv_header_locale_has_locale_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include locale_t x; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_locale_has_locale_t=yes else gl_cv_header_locale_has_locale_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_locale_has_locale_t" >&5 $as_echo "$gl_cv_header_locale_has_locale_t" >&6; } if test $gl_cv_header_locale_has_locale_t = yes; then gl_cv_header_locale_h_needs_xlocale_h=no else gl_cv_header_locale_h_needs_xlocale_h=yes fi else HAVE_XLOCALE_H=0 gl_cv_header_locale_h_needs_xlocale_h=no fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether struct lconv is properly defined" >&5 $as_echo_n "checking whether struct lconv is properly defined... " >&6; } if ${gl_cv_sys_struct_lconv_ok+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include struct lconv l; int x = sizeof (l.decimal_point); int y = sizeof (l.int_p_cs_precedes); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_sys_struct_lconv_ok=yes else gl_cv_sys_struct_lconv_ok=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_sys_struct_lconv_ok" >&5 $as_echo "$gl_cv_sys_struct_lconv_ok" >&6; } if test $gl_cv_sys_struct_lconv_ok = no; then REPLACE_STRUCT_LCONV=1 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_locale_h='<'locale.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_locale_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'locale.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_locale_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_locale_h gl_cv_next_locale_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_locale_h" >&5 $as_echo "$gl_cv_next_locale_h" >&6; } fi NEXT_LOCALE_H=$gl_cv_next_locale_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'locale.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_locale_h fi NEXT_AS_FIRST_DIRECTIVE_LOCALE_H=$gl_next_as_first_directive for gl_func in setlocale duplocale; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... 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" >&6; } if ${gl_cv_pthread_rwlock_rdlock_prefer_writer+:} false; then : $as_echo_n "(cached) " >&6 else save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" if test "$cross_compiling" = yes; then : gl_cv_pthread_rwlock_rdlock_prefer_writer="guessing yes" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define SUCCEED() exit (0) #define FAILURE() exit (1) #define UNEXPECTED(n) (exit (10 + (n))) /* The main thread creates the waiting writer and the requesting reader threads in the default way; this guarantees that they have the same priority. We can reuse the main thread as first reader thread. */ static pthread_rwlock_t lock; static pthread_t reader1; static pthread_t writer; static pthread_t reader2; static pthread_t timer; /* Used to pass control from writer to reader2 and from reader2 to timer, as in a relay race. Passing control from one running thread to another running thread is most likely faster than to create the second thread. */ static pthread_mutex_t baton; static void * timer_func (void *ignored) { /* Step 13 (can be before or after step 12): The timer thread takes the baton, then waits a moment to make sure it can tell whether the second reader thread is blocked at step 12. */ if (pthread_mutex_lock (&baton)) UNEXPECTED (13); usleep (100000); /* By the time we get here, it's clear that the second reader thread is blocked at step 12. This is the desired behaviour. */ SUCCEED (); } static void * reader2_func (void *ignored) { int err; /* Step 8 (can be before or after step 7): The second reader thread takes the baton, then waits a moment to make sure the writer thread has reached step 7. */ if (pthread_mutex_lock (&baton)) UNEXPECTED (8); usleep (100000); /* Step 9: The second reader thread requests the lock. */ err = pthread_rwlock_tryrdlock (&lock); if (err == 0) FAILURE (); else if (err != EBUSY) UNEXPECTED (9); /* Step 10: Launch a timer, to test whether the next call blocks. */ if (pthread_create (&timer, NULL, timer_func, NULL)) UNEXPECTED (10); /* Step 11: Release the baton. */ if (pthread_mutex_unlock (&baton)) UNEXPECTED (11); /* Step 12: The second reader thread requests the lock. */ err = pthread_rwlock_rdlock (&lock); if (err == 0) FAILURE (); else UNEXPECTED (12); } static void * writer_func (void *ignored) { /* Step 4: Take the baton, so that the second reader thread does not go ahead too early. */ if (pthread_mutex_lock (&baton)) UNEXPECTED (4); /* Step 5: Create the second reader thread. */ if (pthread_create (&reader2, NULL, reader2_func, NULL)) UNEXPECTED (5); /* Step 6: Release the baton. */ if (pthread_mutex_unlock (&baton)) UNEXPECTED (6); /* Step 7: The writer thread requests the lock. */ if (pthread_rwlock_wrlock (&lock)) UNEXPECTED (7); return NULL; } int main () { reader1 = pthread_self (); /* Step 1: The main thread initializes the lock and the baton. */ if (pthread_rwlock_init (&lock, NULL)) UNEXPECTED (1); if (pthread_mutex_init (&baton, NULL)) UNEXPECTED (1); /* Step 2: The main thread acquires the lock as a reader. */ if (pthread_rwlock_rdlock (&lock)) UNEXPECTED (2); /* Step 3: Create the writer thread. */ if (pthread_create (&writer, NULL, writer_func, NULL)) UNEXPECTED (3); /* Job done. Go to sleep. */ for (;;) { sleep (1); } } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_pthread_rwlock_rdlock_prefer_writer=yes else gl_cv_pthread_rwlock_rdlock_prefer_writer=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi LIBS="$save_LIBS" fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_pthread_rwlock_rdlock_prefer_writer" >&5 $as_echo "$gl_cv_pthread_rwlock_rdlock_prefer_writer" >&6; } case "$gl_cv_pthread_rwlock_rdlock_prefer_writer" in *yes) $as_echo "#define HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER 1" >>confdefs.h ;; esac fi # glibc defines PTHREAD_MUTEX_RECURSIVE as enum, not as a macro. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #if __FreeBSD__ == 4 error "No, in FreeBSD 4.0 recursive mutexes actually don't work." #elif (defined __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ \ && __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ < 1070) error "No, in Mac OS X < 10.7 recursive mutexes actually don't work." #else int x = (int)PTHREAD_MUTEX_RECURSIVE; return !x; #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : $as_echo "#define HAVE_PTHREAD_MUTEX_RECURSIVE 1" >>confdefs.h fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi : cat >>confdefs.h <<_ACEOF #define GNULIB_LOCK 1 _ACEOF for ac_header in stdlib.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdlib.h" "ac_cv_header_stdlib_h" "$ac_includes_default" if test "x$ac_cv_header_stdlib_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDLIB_H 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for GNU libc compatible malloc" >&5 $as_echo_n "checking for GNU libc compatible malloc... " >&6; } if ${ac_cv_func_malloc_0_nonnull+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on platforms where we know the result. *-gnu* | freebsd* | netbsd* | openbsd* \ | hpux* | solaris* | cygwin* | mingw*) ac_cv_func_malloc_0_nonnull=yes ;; # If we don't know, assume the worst. *) ac_cv_func_malloc_0_nonnull=no ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined STDC_HEADERS || defined HAVE_STDLIB_H # include #else char *malloc (); #endif int main () { char *p = malloc (0); int result = !p; free (p); return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_func_malloc_0_nonnull=yes else ac_cv_func_malloc_0_nonnull=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_func_malloc_0_nonnull" >&5 $as_echo "$ac_cv_func_malloc_0_nonnull" >&6; } if test $ac_cv_func_malloc_0_nonnull = yes; then : $as_echo "#define HAVE_MALLOC_GNU 1" >>confdefs.h else $as_echo "#define HAVE_MALLOC_GNU 0" >>confdefs.h REPLACE_MALLOC=1 fi if test $REPLACE_MALLOC = 1; then gl_LIBOBJS="$gl_LIBOBJS malloc.$ac_objext" fi cat >>confdefs.h <<_ACEOF #define GNULIB_MALLOC_GNU 1 _ACEOF if test $gl_cv_func_malloc_posix = yes; then $as_echo "#define HAVE_MALLOC_POSIX 1" >>confdefs.h else REPLACE_MALLOC=1 fi if test $REPLACE_MALLOC = 1; then gl_LIBOBJS="$gl_LIBOBJS malloc.$ac_objext" fi GNULIB_MALLOC_POSIX=1 $as_echo "#define GNULIB_TEST_MALLOC_POSIX 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_math_h='<'math.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_math_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_math_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'math.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_math_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_math_h gl_cv_next_math_h='"'$gl_header'"' else gl_cv_next_math_h='<'math.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_math_h" >&5 $as_echo "$gl_cv_next_math_h" >&6; } fi NEXT_MATH_H=$gl_cv_next_math_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'math.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_math_h fi NEXT_AS_FIRST_DIRECTIVE_MATH_H=$gl_next_as_first_directive { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether NAN macro works" >&5 $as_echo_n "checking whether NAN macro works... " >&6; } if ${gl_cv_header_math_nan_works+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { /* Solaris 10 has a broken definition of NAN. Other platforms fail to provide NAN, or provide it only in C99 mode; this test only needs to fail when NAN is provided but wrong. */ float f = 1.0f; #ifdef NAN f = NAN; #endif return f == 0; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_math_nan_works=yes else gl_cv_header_math_nan_works=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_math_nan_works" >&5 $as_echo "$gl_cv_header_math_nan_works" >&6; } if test $gl_cv_header_math_nan_works = no; then REPLACE_NAN=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether HUGE_VAL works" >&5 $as_echo_n "checking whether HUGE_VAL works... " >&6; } if ${gl_cv_header_math_huge_val_works+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { /* Solaris 10 has a broken definition of HUGE_VAL. */ double d = HUGE_VAL; return d == 0; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_math_huge_val_works=yes else gl_cv_header_math_huge_val_works=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_math_huge_val_works" >&5 $as_echo "$gl_cv_header_math_huge_val_works" >&6; } if test $gl_cv_header_math_huge_val_works = no; then REPLACE_HUGE_VAL=1 fi for gl_func in acosf acosl asinf asinl atanf atanl cbrt cbrtf cbrtl ceilf ceill copysign copysignf copysignl cosf cosl coshf expf expl exp2 exp2f exp2l expm1 expm1f expm1l fabsf fabsl floorf floorl fma fmaf fmal fmod fmodf fmodl frexpf frexpl hypotf hypotl ilogb ilogbf ilogbl ldexpf ldexpl log logf logl log10 log10f log10l log1p log1pf log1pl log2 log2f log2l logb logbf logbl modf modff modfl powf remainder remainderf remainderl rint rintf rintl round roundf roundl sinf sinl sinhf sqrtf sqrtl tanf tanl tanhf trunc truncf truncl; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $ac_cv_func_mbsinit = yes && test $ac_cv_func_mbrtowc = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles incomplete characters" >&5 $as_echo_n "checking whether mbrtowc handles incomplete characters... " >&6; } if ${gl_cv_func_mbrtowc_incomplete_state+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on AIX and OSF/1. aix* | osf*) gl_cv_func_mbrtowc_incomplete_state="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_incomplete_state="guessing yes" ;; esac if test $LOCALE_JA != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_incomplete_state=yes else gl_cv_func_mbrtowc_incomplete_state=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_incomplete_state" >&5 $as_echo "$gl_cv_func_mbrtowc_incomplete_state" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works as well as mbtowc" >&5 $as_echo_n "checking whether mbrtowc works as well as mbtowc... " >&6; } if ${gl_cv_func_mbrtowc_sanitycheck+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris 8. solaris2.8) gl_cv_func_mbrtowc_sanitycheck="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_sanitycheck="guessing yes" ;; esac if test $LOCALE_ZH_CN != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_sanitycheck=yes else gl_cv_func_mbrtowc_sanitycheck=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_sanitycheck" >&5 $as_echo "$gl_cv_func_mbrtowc_sanitycheck" >&6; } REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi if test $ac_cv_func_mbrtowc = no; then HAVE_MBRTOWC=0 ac_fn_c_check_decl "$LINENO" "mbrtowc" "ac_cv_have_decl_mbrtowc" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_mbrtowc" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_MBRTOWC $ac_have_decl _ACEOF if test $ac_cv_have_decl_mbrtowc = yes; then REPLACE_MBRTOWC=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBRTOWC=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles a NULL pwc argument" >&5 $as_echo_n "checking whether mbrtowc handles a NULL pwc argument... " >&6; } if ${gl_cv_func_mbrtowc_null_arg1+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on Solaris. solaris*) gl_cv_func_mbrtowc_null_arg1="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg1="guessing yes" ;; esac if test $LOCALE_FR_UTF8 != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "\303\237er"; mbstate_t state; wchar_t wc; size_t ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 5, &state); if (ret != 2) result |= 1; if (!mbsinit (&state)) result |= 2; memset (&state, '\0', sizeof (mbstate_t)); ret = mbrtowc (NULL, input, 5, &state); if (ret != 2) /* Solaris 7 fails here: ret is -1. */ result |= 4; if (!mbsinit (&state)) result |= 8; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_null_arg1=yes else gl_cv_func_mbrtowc_null_arg1=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_null_arg1" >&5 $as_echo "$gl_cv_func_mbrtowc_null_arg1" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles a NULL string argument" >&5 $as_echo_n "checking whether mbrtowc handles a NULL string argument... " >&6; } if ${gl_cv_func_mbrtowc_null_arg2+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on OSF/1. osf*) gl_cv_func_mbrtowc_null_arg2="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg2="guessing yes" ;; esac if test $LOCALE_FR_UTF8 != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { mbstate_t state; wchar_t wc; int ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; mbrtowc (&wc, NULL, 5, &state); /* Check that wc was not modified. */ if (wc != (wchar_t) 0xBADFACE) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_null_arg2=yes else gl_cv_func_mbrtowc_null_arg2=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_null_arg2" >&5 $as_echo "$gl_cv_func_mbrtowc_null_arg2" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc has a correct return value" >&5 $as_echo_n "checking whether mbrtowc has a correct return value... " >&6; } if ${gl_cv_func_mbrtowc_retval+:} false; then : $as_echo_n "(cached) " >&6 else case "$host_os" in # Guess no on HP-UX, Solaris, native Windows. hpux* | solaris* | mingw*) gl_cv_func_mbrtowc_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_retval="guessing yes" ;; esac if test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none \ || { case "$host_os" in mingw*) true;; *) false;; esac; }; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; int found_some_locale = 0; /* This fails on Solaris. */ if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "B\303\274\303\237er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 1) result |= 1; } found_some_locale = 1; } /* This fails on HP-UX 11.11. */ if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 2) result |= 2; } found_some_locale = 1; } /* This fails on native Windows. */ if (setlocale (LC_ALL, "Japanese_Japan.932") != NULL) { char input[] = "<\223\372\226\173\214\352>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 4; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_Taiwan.950") != NULL) { char input[] = "<\244\351\245\273\273\171>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 8; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_China.936") != NULL) { char input[] = "<\310\325\261\276\325\132>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 16; } found_some_locale = 1; } return (found_some_locale ? result : 77); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_retval=yes else if test $? != 77; then gl_cv_func_mbrtowc_retval=no fi fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_retval" >&5 $as_echo "$gl_cv_func_mbrtowc_retval" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc returns 0 when parsing a NUL character" >&5 $as_echo_n "checking whether mbrtowc returns 0 when parsing a NUL character... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8 and 9. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, "", 1, &state) != 0) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_nul_retval=yes else gl_cv_func_mbrtowc_nul_retval=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_nul_retval" >&5 $as_echo "$gl_cv_func_mbrtowc_nul_retval" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works on empty input" >&5 $as_echo_n "checking whether mbrtowc works on empty input... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_incomplete_state=yes else gl_cv_func_mbrtowc_incomplete_state=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_incomplete_state" >&5 $as_echo "$gl_cv_func_mbrtowc_incomplete_state" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works as well as mbtowc" >&5 $as_echo_n "checking whether mbrtowc works as well as mbtowc... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_sanitycheck=yes else gl_cv_func_mbrtowc_sanitycheck=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_sanitycheck" >&5 $as_echo "$gl_cv_func_mbrtowc_sanitycheck" >&6; } REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi if test $ac_cv_func_mbsinit = no; then HAVE_MBSINIT=0 ac_fn_c_check_decl "$LINENO" "mbsinit" "ac_cv_have_decl_mbsinit" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_mbsinit" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_MBSINIT $ac_have_decl _ACEOF if test $ac_cv_have_decl_mbsinit = yes; then REPLACE_MBSINIT=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBSINIT=1 else case "$host_os" in mingw*) REPLACE_MBSINIT=1 ;; esac fi fi if test $HAVE_MBSINIT = 0 || test $REPLACE_MBSINIT = 1; then gl_LIBOBJS="$gl_LIBOBJS mbsinit.$ac_objext" : fi GNULIB_MBSINIT=1 $as_echo "#define GNULIB_TEST_MBSINIT 1" >>confdefs.h GNULIB_MBSPBRK=1 $as_echo "#define GNULIB_TEST_MBSPBRK 1" >>confdefs.h GNULIB_MBSSPN=1 $as_echo "#define GNULIB_TEST_MBSSPN 1" >>confdefs.h GNULIB_MBSTOK_R=1 $as_echo "#define GNULIB_TEST_MBSTOK_R 1" >>confdefs.h if false; then REPLACE_MBTOWC=1 fi if test $REPLACE_MBTOWC = 1; then gl_LIBOBJS="$gl_LIBOBJS mbtowc.$ac_objext" : fi GNULIB_MBTOWC=1 $as_echo "#define GNULIB_TEST_MBTOWC 1" >>confdefs.h : if test $HAVE_MEMCHR = 0 || test $REPLACE_MEMCHR = 1; then gl_LIBOBJS="$gl_LIBOBJS memchr.$ac_objext" for ac_header in bp-sym.h do : ac_fn_c_check_header_mongrel "$LINENO" "bp-sym.h" "ac_cv_header_bp_sym_h" "$ac_includes_default" if test "x$ac_cv_header_bp_sym_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_BP_SYM_H 1 _ACEOF fi done fi GNULIB_MEMCHR=1 $as_echo "#define GNULIB_TEST_MEMCHR 1" >>confdefs.h for ac_func in mempcpy do : ac_fn_c_check_func "$LINENO" "mempcpy" "ac_cv_func_mempcpy" if test "x$ac_cv_func_mempcpy" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_MEMPCPY 1 _ACEOF fi done if test $ac_cv_func_mempcpy = no; then HAVE_MEMPCPY=0 fi if test $HAVE_MEMPCPY = 0; then gl_LIBOBJS="$gl_LIBOBJS mempcpy.$ac_objext" : fi GNULIB_MEMPCPY=1 $as_echo "#define GNULIB_TEST_MEMPCPY 1" >>confdefs.h if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then gl_LIBOBJS="$gl_LIBOBJS msvc-inval.$ac_objext" fi if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then gl_LIBOBJS="$gl_LIBOBJS msvc-nothrow.$ac_objext" fi cat >>confdefs.h <<_ACEOF #define GNULIB_MSVC_NOTHROW 1 _ACEOF if test $ac_cv_func_nl_langinfo = yes; then # On Irix 6.5, YESEXPR is defined, but nl_langinfo(YESEXPR) is broken. { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether YESEXPR works" >&5 $as_echo_n "checking whether YESEXPR works... 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" >&6; } if ${gl_cv_func_sched_getaffinity3+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { sched_getaffinity (0, 0, (cpu_set_t *) 0); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_sched_getaffinity3=yes else gl_cv_func_sched_getaffinity3=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_sched_getaffinity3" >&5 $as_echo "$gl_cv_func_sched_getaffinity3" >&6; } if test $gl_cv_func_sched_getaffinity3 = yes; then $as_echo "#define HAVE_SCHED_GETAFFINITY_LIKE_GLIBC 1" >>confdefs.h fi fi for ac_func in rawmemchr do : ac_fn_c_check_func "$LINENO" "rawmemchr" "ac_cv_func_rawmemchr" if test "x$ac_cv_func_rawmemchr" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_RAWMEMCHR 1 _ACEOF fi done if test $ac_cv_func_rawmemchr = no; then HAVE_RAWMEMCHR=0 fi if test $HAVE_RAWMEMCHR = 0; then gl_LIBOBJS="$gl_LIBOBJS rawmemchr.$ac_objext" : fi GNULIB_RAWMEMCHR=1 $as_echo "#define GNULIB_TEST_RAWMEMCHR 1" >>confdefs.h # Check whether --with-included-regex was given. if test "${with_included_regex+set}" = set; then : withval=$with_included_regex; fi case $with_included_regex in #( yes|no) ac_use_included_regex=$with_included_regex ;; '') # If the system regex support is good enough that it passes the # following run test, then default to *not* using the included regex.c. # If cross compiling, assume the test would fail and use the included # regex.c. { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working re_compile_pattern" >&5 $as_echo_n "checking for working re_compile_pattern... " >&6; } if ${gl_cv_func_re_compile_pattern_working+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess no on native Windows. mingw*) gl_cv_func_re_compile_pattern_working="guessing no" ;; # Otherwise, assume it is not working. *) gl_cv_func_re_compile_pattern_working="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #if defined M_CHECK_ACTION || HAVE_DECL_ALARM # include # include #endif #if HAVE_MALLOC_H # include #endif #ifdef M_CHECK_ACTION /* Exit with distinguishable exit code. */ static void sigabrt_no_core (int sig) { raise (SIGTERM); } #endif int main () { int result = 0; static struct re_pattern_buffer regex; unsigned char folded_chars[UCHAR_MAX + 1]; int i; const char *s; struct re_registers regs; /* Some builds of glibc go into an infinite loop on this test. Use alarm to force death, and mallopt to avoid malloc recursion in diagnosing the corrupted heap. */ #if HAVE_DECL_ALARM signal (SIGALRM, SIG_DFL); alarm (2); #endif #ifdef M_CHECK_ACTION signal (SIGABRT, sigabrt_no_core); mallopt (M_CHECK_ACTION, 2); #endif if (setlocale (LC_ALL, "en_US.UTF-8")) { { /* https://sourceware.org/ml/libc-hacker/2006-09/msg00008.html This test needs valgrind to catch the bug on Debian GNU/Linux 3.1 x86, but it might catch the bug better on other platforms and it shouldn't hurt to try the test here. */ static char const pat[] = "insert into"; static char const data[] = "\xFF\0\x12\xA2\xAA\xC4\xB1,K\x12\xC4\xB1*\xACK"; re_set_syntax (RE_SYNTAX_GREP | RE_HAT_LISTS_NOT_NEWLINE | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else if (re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, ®s) != -1) result |= 1; regfree (®ex); } { /* This test is from glibc bug 15078. The test case is from Andreas Schwab in . */ static char const pat[] = "[^x]x"; static char const data[] = /* */ "\xe1\x80\x80" "\xe1\x80\xbb" "\xe1\x80\xbd" "\xe1\x80\x94" "\xe1\x80\xba" "\xe1\x80\xaf" "\xe1\x80\x95" "\xe1\x80\xba" "x"; re_set_syntax (0); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { i = re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, 0); if (i != 0 && i != 21) result |= 1; } regfree (®ex); } if (! setlocale (LC_ALL, "C")) return 1; } /* This test is from glibc bug 3957, reported by Andrew Mackey. */ re_set_syntax (RE_SYNTAX_EGREP | RE_HAT_LISTS_NOT_NEWLINE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[^x]b", 6, ®ex); if (s) result |= 2; /* This should fail, but succeeds for glibc-2.5. */ else if (re_search (®ex, "a\nb", 3, 0, 3, ®s) != -1) result |= 2; /* This regular expression is from Spencer ere test number 75 in grep-2.3. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP); memset (®ex, 0, sizeof regex); for (i = 0; i <= UCHAR_MAX; i++) folded_chars[i] = i; regex.translate = folded_chars; s = re_compile_pattern ("a[[:]:]]b\n", 11, ®ex); /* This should fail with _Invalid character class name_ error. */ if (!s) result |= 4; /* Ensure that [b-a] is diagnosed as invalid, when using RE_NO_EMPTY_RANGES. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP | RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[b-a]", 6, ®ex); if (s == 0) result |= 8; /* This should succeed, but does not for glibc-2.1.3. */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("{1", 2, ®ex); if (s) result |= 8; /* The following example is derived from a problem report against gawk from Jorge Stolfi . */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[an\371]*n", 7, ®ex); if (s) result |= 8; /* This should match, but does not for glibc-2.2.1. */ else if (re_match (®ex, "an", 2, 0, ®s) != 2) result |= 8; memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 8; /* glibc-2.2.93 does not work with a negative RANGE argument. */ else if (re_search (®ex, "wxy", 3, 2, -2, ®s) != 1) result |= 8; /* The version of regex.c in older versions of gnulib ignored RE_ICASE. Detect that problem too. */ re_set_syntax (RE_SYNTAX_EMACS | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 16; else if (re_search (®ex, "WXY", 3, 0, 3, ®s) < 0) result |= 16; /* Catch a bug reported by Vin Shelton in https://lists.gnu.org/r/bug-coreutils/2007-06/msg00089.html */ re_set_syntax (RE_SYNTAX_POSIX_BASIC & ~RE_CONTEXT_INVALID_DUP & ~RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[[:alnum:]_-]\\\\+$", 16, ®ex); if (s) result |= 32; /* REG_STARTEND was added to glibc on 2004-01-15. Reject older versions. */ if (! REG_STARTEND) result |= 64; #if 0 /* It would be nice to reject hosts whose regoff_t values are too narrow (including glibc on hosts with 64-bit ptrdiff_t and 32-bit int), but we should wait until glibc implements this feature. Otherwise, support for equivalence classes and multibyte collation symbols would always be broken except when compiling --without-included-regex. */ if (sizeof (regoff_t) < sizeof (ptrdiff_t) || sizeof (regoff_t) < sizeof (ssize_t)) result |= 64; #endif return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_re_compile_pattern_working=yes else gl_cv_func_re_compile_pattern_working=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_re_compile_pattern_working" >&5 $as_echo "$gl_cv_func_re_compile_pattern_working" >&6; } case "$gl_cv_func_re_compile_pattern_working" in #( *yes) ac_use_included_regex=no;; #( *no) ac_use_included_regex=yes;; esac ;; *) as_fn_error $? "Invalid value for --with-included-regex: $with_included_regex" "$LINENO" 5 ;; esac if test $ac_use_included_regex = yes; then $as_echo "#define _REGEX_INCLUDE_LIMITS_H 1" >>confdefs.h $as_echo "#define _REGEX_LARGE_OFFSETS 1" >>confdefs.h $as_echo "#define re_syntax_options rpl_re_syntax_options" >>confdefs.h $as_echo "#define re_set_syntax rpl_re_set_syntax" >>confdefs.h $as_echo "#define re_compile_pattern rpl_re_compile_pattern" >>confdefs.h $as_echo "#define re_compile_fastmap rpl_re_compile_fastmap" >>confdefs.h $as_echo "#define re_search rpl_re_search" >>confdefs.h $as_echo "#define re_search_2 rpl_re_search_2" >>confdefs.h $as_echo "#define re_match rpl_re_match" >>confdefs.h $as_echo "#define re_match_2 rpl_re_match_2" >>confdefs.h $as_echo "#define re_set_registers rpl_re_set_registers" >>confdefs.h $as_echo "#define re_comp rpl_re_comp" >>confdefs.h $as_echo "#define re_exec rpl_re_exec" >>confdefs.h $as_echo "#define regcomp rpl_regcomp" >>confdefs.h $as_echo "#define regexec rpl_regexec" >>confdefs.h $as_echo "#define regerror rpl_regerror" >>confdefs.h $as_echo "#define regfree rpl_regfree" >>confdefs.h fi if test $ac_use_included_regex = yes; then gl_LIBOBJS="$gl_LIBOBJS regex.$ac_objext" for ac_header in libintl.h do : ac_fn_c_check_header_mongrel "$LINENO" "libintl.h" "ac_cv_header_libintl_h" "$ac_includes_default" if test "x$ac_cv_header_libintl_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_LIBINTL_H 1 _ACEOF fi done ac_fn_c_check_decl "$LINENO" "isblank" "ac_cv_have_decl_isblank" "#include " if test "x$ac_cv_have_decl_isblank" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_ISBLANK $ac_have_decl _ACEOF fi for ac_header in stdint.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdint.h" "ac_cv_header_stdint_h" "$ac_includes_default" if test "x$ac_cv_header_stdint_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDINT_H 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for SIZE_MAX" >&5 $as_echo_n "checking for SIZE_MAX... 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This catches GCC bug 52023 . */ #ifdef __cplusplus template struct alignof_helper { char a; t b; }; # define ao(type) offsetof (alignof_helper, b) #else # define ao(type) offsetof (struct { char a; type b; }, b) #endif char test_double[ao (double) % _Alignof (double) == 0 ? 1 : -1]; char test_long[ao (long int) % _Alignof (long int) == 0 ? 1 : -1]; char test_alignof[alignof (double) == _Alignof (double) ? 1 : -1]; /* Test _Alignas only on platforms where gnulib can help. */ #if \ ((defined __cplusplus && 201103 <= __cplusplus) \ || (defined __APPLE__ && defined __MACH__ \ ? 4 < __GNUC__ + (1 <= __GNUC_MINOR__) \ : __GNUC__) \ || (__ia64 && (61200 <= __HP_cc || 61200 <= __HP_aCC)) \ || __ICC || 0x590 <= __SUNPRO_C || 0x0600 <= __xlC__ \ || 1300 <= _MSC_VER) struct alignas_test { char c; char alignas (8) alignas_8; }; char test_alignas[offsetof (struct alignas_test, alignas_8) == 8 ? 1 : -1]; #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_header_working_stdalign_h=yes else gl_cv_header_working_stdalign_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_header_working_stdalign_h" >&5 $as_echo "$gl_cv_header_working_stdalign_h" >&6; } if test $gl_cv_header_working_stdalign_h = yes; then STDALIGN_H='' else STDALIGN_H='stdalign.h' fi if test -n "$STDALIGN_H"; then GL_GENERATE_STDALIGN_H_TRUE= GL_GENERATE_STDALIGN_H_FALSE='#' else GL_GENERATE_STDALIGN_H_TRUE='#' GL_GENERATE_STDALIGN_H_FALSE= fi # Define two additional variables used in the Makefile substitution. if test "$ac_cv_header_stdbool_h" = yes; then STDBOOL_H='' else STDBOOL_H='stdbool.h' fi if test -n "$STDBOOL_H"; then GL_GENERATE_STDBOOL_H_TRUE= GL_GENERATE_STDBOOL_H_FALSE='#' else GL_GENERATE_STDBOOL_H_TRUE='#' GL_GENERATE_STDBOOL_H_FALSE= fi if test "$ac_cv_type__Bool" = yes; then HAVE__BOOL=1 else HAVE__BOOL=0 fi STDDEF_H= ac_fn_c_check_type "$LINENO" "max_align_t" "ac_cv_type_max_align_t" "#include " if test "x$ac_cv_type_max_align_t" = xyes; then : else HAVE_MAX_ALIGN_T=0; STDDEF_H=stddef.h fi if test $gt_cv_c_wchar_t = no; then HAVE_WCHAR_T=0 STDDEF_H=stddef.h fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether NULL can be used in arbitrary expressions" >&5 $as_echo_n "checking whether NULL can be used in arbitrary expressions... 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HP-UX 11.31 parses inf, but mistakenly sets errno. */ const char *string = "inf"; char *term; double value; errno = 0; value = strtod (string, &term); if (value != HUGE_VAL || term != (string + 3) || errno) result |= 16; } { /* glibc 2.7 and cygwin 1.5.24 misparse "nan()". */ const char *string = "nan()"; char *term; double value = strtod (string, &term); if (numeric_equal (value, value) || term != (string + 5)) result |= 32; } { /* darwin 10.6.1 misparses "nan(". */ const char *string = "nan("; char *term; double value = strtod (string, &term); if (numeric_equal (value, value) || term != (string + 3)) result |= 64; } return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_strtod_works=yes else gl_cv_func_strtod_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_strtod_works" >&5 $as_echo "$gl_cv_func_strtod_works" >&6; } case "$gl_cv_func_strtod_works" in *yes) ;; *) REPLACE_STRTOD=1 ;; esac fi if test $HAVE_STRTOD = 0 || test $REPLACE_STRTOD = 1; then gl_LIBOBJS="$gl_LIBOBJS strtod.$ac_objext" if test $gl_cv_func_ldexp_no_libm = yes; then $as_echo "#define HAVE_LDEXP_IN_LIBC 1" >>confdefs.h fi fi GNULIB_STRTOD=1 $as_echo "#define GNULIB_TEST_STRTOD 1" >>confdefs.h for ac_func in strtok_r do : ac_fn_c_check_func "$LINENO" "strtok_r" "ac_cv_func_strtok_r" if test "x$ac_cv_func_strtok_r" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRTOK_R 1 _ACEOF fi done if test $ac_cv_func_strtok_r = yes; then HAVE_STRTOK_R=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether strtok_r works" >&5 $as_echo_n "checking whether strtok_r works... 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" >&6; } if ${gl_cv_next_sysexits_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sysexits_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sysexits.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sysexits_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sysexits_h gl_cv_next_sysexits_h='"'$gl_header'"' else gl_cv_next_sysexits_h='<'sysexits.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sysexits_h" >&5 $as_echo "$gl_cv_next_sysexits_h" >&6; } fi NEXT_SYSEXITS_H=$gl_cv_next_sysexits_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sysexits.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sysexits_h fi NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H=$gl_next_as_first_directive cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { switch (0) { case EX_OK: case EX_USAGE: case EX_DATAERR: case EX_NOINPUT: case EX_NOUSER: case EX_NOHOST: case EX_UNAVAILABLE: case EX_SOFTWARE: case EX_OSERR: case EX_OSFILE: case EX_CANTCREAT: case EX_IOERR: case EX_TEMPFAIL: case EX_PROTOCOL: case EX_NOPERM: case EX_CONFIG: break; } ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : SYSEXITS_H= else SYSEXITS_H=sysexits.h fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else HAVE_SYSEXITS_H=0 SYSEXITS_H=sysexits.h fi if test -n "$SYSEXITS_H"; then GL_GENERATE_SYSEXITS_H_TRUE= GL_GENERATE_SYSEXITS_H_FALSE='#' else GL_GENERATE_SYSEXITS_H_TRUE='#' GL_GENERATE_SYSEXITS_H_FALSE= fi if test $gl_cv_have_include_next = yes; then gl_cv_next_unistd_h='<'unistd.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_unistd_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_unistd_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'unistd.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_unistd_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_unistd_h gl_cv_next_unistd_h='"'$gl_header'"' else gl_cv_next_unistd_h='<'unistd.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_unistd_h" >&5 $as_echo "$gl_cv_next_unistd_h" >&6; } fi NEXT_UNISTD_H=$gl_cv_next_unistd_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'unistd.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_unistd_h fi NEXT_AS_FIRST_DIRECTIVE_UNISTD_H=$gl_next_as_first_directive if test $ac_cv_header_unistd_h = yes; then HAVE_UNISTD_H=1 else HAVE_UNISTD_H=0 fi for gl_func in chdir chown dup dup2 dup3 environ euidaccess faccessat fchdir fchownat fdatasync fsync ftruncate getcwd getdomainname getdtablesize getgroups gethostname getlogin getlogin_r getpagesize getusershell setusershell endusershell group_member isatty lchown link linkat lseek pipe pipe2 pread pwrite readlink readlinkat rmdir sethostname sleep symlink symlinkat truncate ttyname_r unlink unlinkat usleep; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if HAVE_UNISTD_H # include #endif /* Some systems declare various items in the wrong headers. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include # endif #endif int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if { test "$HAVE_LIBUNISTRING" != yes \ || { test $LIBUNISTRING_VERSION_MAJOR -lt 0 \ || { test $LIBUNISTRING_VERSION_MAJOR -eq 0 \ && { test $LIBUNISTRING_VERSION_MINOR -lt 9 \ || { test $LIBUNISTRING_VERSION_MINOR -eq 9 \ && test $LIBUNISTRING_VERSION_SUBMINOR -lt 4 } } } } }; then LIBUNISTRING_UNITYPES_H='unitypes.h' else LIBUNISTRING_UNITYPES_H= fi if { test "$HAVE_LIBUNISTRING" != yes \ || { test $LIBUNISTRING_VERSION_MAJOR -lt 0 \ || { test $LIBUNISTRING_VERSION_MAJOR -eq 0 \ && { test $LIBUNISTRING_VERSION_MINOR -lt 9 \ || { test $LIBUNISTRING_VERSION_MINOR -eq 9 \ && test $LIBUNISTRING_VERSION_SUBMINOR -lt 4 } } } } }; then LIBUNISTRING_UNIWIDTH_H='uniwidth.h' else LIBUNISTRING_UNIWIDTH_H= fi if { test "$HAVE_LIBUNISTRING" != yes \ || { test $LIBUNISTRING_VERSION_MAJOR -lt 0 \ || { test $LIBUNISTRING_VERSION_MAJOR -eq 0 \ && { test $LIBUNISTRING_VERSION_MINOR -lt 9 \ || { test $LIBUNISTRING_VERSION_MINOR -eq 9 \ && test $LIBUNISTRING_VERSION_SUBMINOR -lt 8 } } } } }; then LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH_TRUE= LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH_FALSE='#' else LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH_TRUE='#' LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH_FALSE= fi if test $ac_cv_func_vasnprintf = no; then gl_LIBOBJS="$gl_LIBOBJS vasnprintf.$ac_objext" gl_LIBOBJS="$gl_LIBOBJS printf-args.$ac_objext" gl_LIBOBJS="$gl_LIBOBJS printf-parse.$ac_objext" gl_LIBOBJS="$gl_LIBOBJS asnprintf.$ac_objext" if test $ac_cv_func_vasnprintf = yes; then $as_echo "#define REPLACE_VASNPRINTF 1" >>confdefs.h fi ac_fn_c_check_type "$LINENO" "ptrdiff_t" "ac_cv_type_ptrdiff_t" "$ac_includes_default" if test "x$ac_cv_type_ptrdiff_t" = xyes; then : else $as_echo "#define ptrdiff_t long" >>confdefs.h fi fi gl_cv_func_vsnprintf_usable=no for ac_func in vsnprintf do : ac_fn_c_check_func "$LINENO" "vsnprintf" "ac_cv_func_vsnprintf" if test "x$ac_cv_func_vsnprintf" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_VSNPRINTF 1 _ACEOF fi done if test $ac_cv_func_vsnprintf = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether snprintf respects a size of 1" >&5 $as_echo_n "checking whether snprintf respects a size of 1... 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" >&6; } if ${gl_cv_func_printf_positions+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in netbsd[1-3]* | netbsdelf[1-3]* | netbsdaout[1-3]* | netbsdcoff[1-3]*) gl_cv_func_printf_positions="guessing no";; beos*) gl_cv_func_printf_positions="guessing no";; # Guess no on native Windows. mingw* | pw*) gl_cv_func_printf_positions="guessing no";; *) gl_cv_func_printf_positions="guessing yes";; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* The string "%2$d %1$d", with dollar characters protected from the shell's dollar expansion (possibly an autoconf bug). */ static char format[] = { '%', '2', '$', 'd', ' ', '%', '1', '$', 'd', '\0' }; static char buf[100]; int main () { sprintf (buf, format, 33, 55); return (strcmp (buf, "55 33") != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_printf_positions=yes else gl_cv_func_printf_positions=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_printf_positions" >&5 $as_echo "$gl_cv_func_printf_positions" >&6; } case "$gl_cv_func_printf_positions" in *yes) gl_cv_func_vsnprintf_usable=yes ;; esac ;; esac ;; esac fi if test $gl_cv_func_vsnprintf_usable = no; then gl_LIBOBJS="$gl_LIBOBJS vsnprintf.$ac_objext" if test $ac_cv_func_vsnprintf = yes; then REPLACE_VSNPRINTF=1 else if test $ac_cv_have_decl_vsnprintf = yes; then REPLACE_VSNPRINTF=1 fi fi : fi if test $ac_cv_have_decl_vsnprintf = no; then HAVE_DECL_VSNPRINTF=0 fi GNULIB_VSNPRINTF=1 $as_echo "#define GNULIB_TEST_VSNPRINTF 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_wchar_h='<'wchar.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_wchar_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_wchar_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'wchar.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_wchar_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_wchar_h gl_cv_next_wchar_h='"'$gl_header'"' else gl_cv_next_wchar_h='<'wchar.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_wchar_h" >&5 $as_echo "$gl_cv_next_wchar_h" >&6; } fi NEXT_WCHAR_H=$gl_cv_next_wchar_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'wchar.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_wchar_h fi NEXT_AS_FIRST_DIRECTIVE_WCHAR_H=$gl_next_as_first_directive if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi for gl_func in btowc wctob mbsinit mbrtowc mbrlen mbsrtowcs mbsnrtowcs wcrtomb wcsrtombs wcsnrtombs wcwidth wmemchr wmemcmp wmemcpy wmemmove wmemset wcslen wcsnlen wcscpy wcpcpy wcsncpy wcpncpy wcscat wcsncat wcscmp wcsncmp wcscasecmp wcsncasecmp wcscoll wcsxfrm wcsdup wcschr wcsrchr wcscspn wcsspn wcspbrk wcsstr wcstok wcswidth wcsftime ; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $ac_cv_func_mbsinit = yes && test $ac_cv_func_mbrtowc = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc handles incomplete characters" >&5 $as_echo_n "checking whether mbrtowc handles incomplete characters... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_incomplete_state=yes else gl_cv_func_mbrtowc_incomplete_state=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_incomplete_state" >&5 $as_echo "$gl_cv_func_mbrtowc_incomplete_state" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether mbrtowc works as well as mbtowc" >&5 $as_echo_n "checking whether mbrtowc works as well as mbtowc... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 2; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_mbrtowc_sanitycheck=yes else gl_cv_func_mbrtowc_sanitycheck=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_mbrtowc_sanitycheck" >&5 $as_echo "$gl_cv_func_mbrtowc_sanitycheck" >&6; } REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi if test $ac_cv_func_wcrtomb = no; then HAVE_WCRTOMB=0 ac_fn_c_check_decl "$LINENO" "wcrtomb" "ac_cv_have_decl_wcrtomb" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_wcrtomb" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_WCRTOMB $ac_have_decl _ACEOF if test $ac_cv_have_decl_wcrtomb = yes; then REPLACE_WCRTOMB=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_WCRTOMB=1 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether wcrtomb return value is correct" >&5 $as_echo_n "checking whether wcrtomb return value is correct... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 1; } if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 2; } if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 4; } if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 8; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_wcrtomb_retval=yes else gl_cv_func_wcrtomb_retval=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wcrtomb_retval" >&5 $as_echo "$gl_cv_func_wcrtomb_retval" >&6; } case "$gl_cv_func_wcrtomb_retval" in *yes) ;; *) REPLACE_WCRTOMB=1 ;; esac fi fi if test $HAVE_WCRTOMB = 0 || test $REPLACE_WCRTOMB = 1; then gl_LIBOBJS="$gl_LIBOBJS wcrtomb.$ac_objext" : fi GNULIB_WCRTOMB=1 $as_echo "#define GNULIB_TEST_WCRTOMB 1" >>confdefs.h if test $ac_cv_func_iswcntrl = yes; then HAVE_ISWCNTRL=1 else HAVE_ISWCNTRL=0 fi if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_wctype_h='<'wctype.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_wctype_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_wctype_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'wctype.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_wctype_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_wctype_h gl_cv_next_wctype_h='"'$gl_header'"' else gl_cv_next_wctype_h='<'wctype.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_wctype_h" >&5 $as_echo "$gl_cv_next_wctype_h" >&6; } fi NEXT_WCTYPE_H=$gl_cv_next_wctype_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'wctype.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_wctype_h fi NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H=$gl_next_as_first_directive if test $ac_cv_header_wctype_h = yes; then if test $ac_cv_func_iswcntrl = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether iswcntrl works" >&5 $as_echo_n "checking whether iswcntrl works... " >&6; } if ${gl_cv_func_iswcntrl_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNU_LIBRARY__ == 1 Linux libc5 i18n is broken. #endif int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_iswcntrl_works="guessing yes" else gl_cv_func_iswcntrl_works="guessing no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { return iswprint ('x') == 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_iswcntrl_works=yes else gl_cv_func_iswcntrl_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_iswcntrl_works" >&5 $as_echo "$gl_cv_func_iswcntrl_works" >&6; } fi HAVE_WCTYPE_H=1 else HAVE_WCTYPE_H=0 fi case "$gl_cv_func_iswcntrl_works" in *yes) REPLACE_ISWCNTRL=0 ;; *) REPLACE_ISWCNTRL=1 ;; esac if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then : fi if test $REPLACE_ISWCNTRL = 1; then REPLACE_TOWLOWER=1 else for ac_func in towlower do : ac_fn_c_check_func "$LINENO" "towlower" "ac_cv_func_towlower" if test "x$ac_cv_func_towlower" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_TOWLOWER 1 _ACEOF fi done if test $ac_cv_func_towlower = yes; then REPLACE_TOWLOWER=0 else ac_fn_c_check_decl "$LINENO" "towlower" "ac_cv_have_decl_towlower" "/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif " if test "x$ac_cv_have_decl_towlower" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_TOWLOWER $ac_have_decl _ACEOF if test $ac_cv_have_decl_towlower = yes; then REPLACE_TOWLOWER=1 else REPLACE_TOWLOWER=0 fi fi fi if test $HAVE_ISWCNTRL = 0 || test $REPLACE_TOWLOWER = 1; then : fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wctype_t" >&5 $as_echo_n "checking for wctype_t... " >&6; } if ${gl_cv_type_wctype_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif wctype_t a; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wctype_t=yes else gl_cv_type_wctype_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wctype_t" >&5 $as_echo "$gl_cv_type_wctype_t" >&6; } if test $gl_cv_type_wctype_t = no; then HAVE_WCTYPE_T=0 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for wctrans_t" >&5 $as_echo_n "checking for wctrans_t... " >&6; } if ${gl_cv_type_wctrans_t+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include wctrans_t a; int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_type_wctrans_t=yes else gl_cv_type_wctrans_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_type_wctrans_t" >&5 $as_echo "$gl_cv_type_wctrans_t" >&6; } if test $gl_cv_type_wctrans_t = no; then HAVE_WCTRANS_T=0 fi for gl_func in wctype iswctype wctrans towctrans ; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done ac_fn_c_check_decl "$LINENO" "wcwidth" "ac_cv_have_decl_wcwidth" " /* AIX 3.2.5 declares wcwidth in . */ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include " if test "x$ac_cv_have_decl_wcwidth" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_WCWIDTH $ac_have_decl _ACEOF if test $ac_cv_have_decl_wcwidth != yes; then HAVE_DECL_WCWIDTH=0 fi if test $ac_cv_func_wcwidth != yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether wcwidth is a macro" >&5 $as_echo_n "checking whether wcwidth is a macro... " >&6; } if ${gl_cv_func_wcwidth_macro+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef wcwidth wchar_header_defines_wcwidth #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "wchar_header_defines_wcwidth" >/dev/null 2>&1; then : gl_cv_func_wcwidth_macro=yes else gl_cv_func_wcwidth_macro=no fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wcwidth_macro" >&5 $as_echo "$gl_cv_func_wcwidth_macro" >&6; } fi if test $ac_cv_func_wcwidth = yes || test $gl_cv_func_wcwidth_macro = yes; then HAVE_WCWIDTH=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether wcwidth works reasonably in UTF-8 locales" >&5 $as_echo_n "checking whether wcwidth works reasonably in UTF-8 locales... 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if !HAVE_DECL_WCWIDTH extern # ifdef __cplusplus "C" # endif int wcwidth (int); #endif int main () { int result = 0; if (setlocale (LC_ALL, "fr_FR.UTF-8") != NULL) { if (wcwidth (0x0301) > 0) result |= 1; if (wcwidth (0x05B0) > 0) result |= 2; if (wcwidth (0x200B) > 0) result |= 4; if (wcwidth (0xFF1A) == 0) result |= 8; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_wcwidth_works=yes else gl_cv_func_wcwidth_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wcwidth_works" >&5 $as_echo "$gl_cv_func_wcwidth_works" >&6; } case "$gl_cv_func_wcwidth_works" in *yes) ;; *no) REPLACE_WCWIDTH=1 ;; esac else HAVE_WCWIDTH=0 fi if test $HAVE_WCWIDTH = 0 || test $REPLACE_WCWIDTH = 1; then gl_LIBOBJS="$gl_LIBOBJS wcwidth.$ac_objext" fi GNULIB_WCWIDTH=1 $as_echo "#define GNULIB_TEST_WCWIDTH 1" >>confdefs.h for ac_header in stdint.h do : ac_fn_c_check_header_mongrel "$LINENO" "stdint.h" "ac_cv_header_stdint_h" "$ac_includes_default" if test "x$ac_cv_header_stdint_h" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STDINT_H 1 _ACEOF fi done # End of code from modules gltests_libdeps= gltests_ltlibdeps= gl_source_base='bootstrapped/tests' gltests_WITNESS=IN_`echo "${PACKAGE-$PACKAGE_TARNAME}" | LC_ALL=C tr abcdefghijklmnopqrstuvwxyz ABCDEFGHIJKLMNOPQRSTUVWXYZ | LC_ALL=C sed -e 's/[^A-Z0-9_]/_/g'`_GNULIB_TESTS gl_module_indicator_condition=$gltests_WITNESS if test "$ac_cv_header_winsock2_h" = yes; then gltests_LIBOBJS="$gltests_LIBOBJS accept.$ac_objext" fi if test "$GNULIB_ACCEPT" != 1; then if test "$GNULIB_ACCEPT" = 0; then GNULIB_ACCEPT=$gl_module_indicator_condition else GNULIB_ACCEPT="($GNULIB_ACCEPT || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_ACCEPT 1" >>confdefs.h if test $ac_cv_header_arpa_inet_h = yes; then HAVE_ARPA_INET_H=1 else HAVE_ARPA_INET_H=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_arpa_inet_h='<'arpa/inet.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... 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" >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* On some systems, this header is not self-consistent. */ #if !(defined __GLIBC__ || defined __UCLIBC__) # include #endif #ifdef __TANDEM # include #endif #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test "$ac_cv_header_winsock2_h" = yes; then gltests_LIBOBJS="$gltests_LIBOBJS bind.$ac_objext" fi if test "$GNULIB_BIND" != 1; then if test "$GNULIB_BIND" = 0; then GNULIB_BIND=$gl_module_indicator_condition else GNULIB_BIND="($GNULIB_BIND || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_BIND 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... 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Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; # if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; # endif return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... 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Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... " >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; # if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; # endif return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a turkish Unicode locale" >&5 $as_echo_n "checking for a turkish Unicode locale... " >&6; } if ${gt_cv_locale_tr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. But BeOS does not implement the Turkish upper-/lowercase mappings. Therefore, let this program return 1 on BeOS. */ /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the tr_TR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the eighth month, the second character (should be U+011F: LATIN SMALL LETTER G WITH BREVE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1992 - 1900; t.tm_mon = 8 - 1; t.tm_mday = 19; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc4 || buf[2] != (char) 0x9f) return 1; /* Check whether the upper-/lowercase mappings are as expected for Turkish. */ if (towupper ('i') != 0x0130 || towlower (0x0130) != 'i' || towupper(0x0131) != 'I' || towlower ('I') != 0x0131) return 1; return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Turkish_Turkey.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=Turkish_Turkey.65001 else # None found. gt_cv_locale_tr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. 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" >&6; } if ${ac_cv_c_bigendian+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_c_bigendian=unknown # See if we're dealing with a universal compiler. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # Check for potential -arch flags. 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(defined _LITTLE_ENDIAN || defined _BIG_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to _BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #ifndef _BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # Compile a test program. if test "$cross_compiling" = yes; then : # Try to guess by grepping values from an object file. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ short int ascii_mm[] = { 0x4249, 0x4765, 0x6E44, 0x6961, 0x6E53, 0x7953, 0 }; short int ascii_ii[] = { 0x694C, 0x5454, 0x656C, 0x6E45, 0x6944, 0x6E61, 0 }; int use_ascii (int i) { return ascii_mm[i] + ascii_ii[i]; } short int ebcdic_ii[] = { 0x89D3, 0xE3E3, 0x8593, 0x95C5, 0x89C4, 0x9581, 0 }; short int ebcdic_mm[] = { 0xC2C9, 0xC785, 0x95C4, 0x8981, 0x95E2, 0xA8E2, 0 }; int use_ebcdic (int i) { return ebcdic_mm[i] + ebcdic_ii[i]; } extern int foo; int main () { return use_ascii (foo) == use_ebcdic (foo); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if grep BIGenDianSyS conftest.$ac_objext >/dev/null; then ac_cv_c_bigendian=yes fi if grep LiTTleEnDian conftest.$ac_objext >/dev/null ; then if test "$ac_cv_c_bigendian" = unknown; then ac_cv_c_bigendian=no else # finding both strings is unlikely to happen, but who knows? ac_cv_c_bigendian=unknown fi fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { /* Are we little or big endian? From Harbison&Steele. */ union { long int l; char c[sizeof (long int)]; } u; u.l = 1; return u.c[sizeof (long int) - 1] == 1; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_c_bigendian=no else ac_cv_c_bigendian=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_c_bigendian" >&5 $as_echo "$ac_cv_c_bigendian" >&6; } case $ac_cv_c_bigendian in #( yes) $as_echo "#define WORDS_BIGENDIAN 1" >>confdefs.h ;; #( no) ;; #( universal) $as_echo "#define AC_APPLE_UNIVERSAL_BUILD 1" >>confdefs.h ;; #( *) as_fn_error $? "unknown endianness presetting ac_cv_c_bigendian=no (or yes) will help" "$LINENO" 5 ;; esac HAVE_IOCTL=1 if test "$ac_cv_header_winsock2_h" = yes; then HAVE_IOCTL=0 else for ac_func in ioctl do : ac_fn_c_check_func "$LINENO" "ioctl" "ac_cv_func_ioctl" if test "x$ac_cv_func_ioctl" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_IOCTL 1 _ACEOF fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for ioctl with POSIX signature" >&5 $as_echo_n "checking for ioctl with POSIX signature... " >&6; } if ${gl_cv_func_ioctl_posix_signature+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include /* On some platforms, ioctl() is declared in . */ #include int main () { extern #ifdef __cplusplus "C" #endif int ioctl (int, int, ...); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_func_ioctl_posix_signature=yes else gl_cv_func_ioctl_posix_signature=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_ioctl_posix_signature" >&5 $as_echo "$gl_cv_func_ioctl_posix_signature" >&6; } if test $gl_cv_func_ioctl_posix_signature != yes; then REPLACE_IOCTL=1 fi fi if test $HAVE_IOCTL = 0 || test $REPLACE_IOCTL = 1; then gltests_LIBOBJS="$gltests_LIBOBJS ioctl.$ac_objext" fi if test "$GNULIB_IOCTL" != 1; then if test "$GNULIB_IOCTL" = 0; then GNULIB_IOCTL=$gl_module_indicator_condition else GNULIB_IOCTL="($GNULIB_IOCTL || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_IOCTL 1" >>confdefs.h if test $ac_cv_func_isblank = no; then HAVE_ISBLANK=0 fi if test $HAVE_ISBLANK = 0; then gltests_LIBOBJS="$gltests_LIBOBJS isblank.$ac_objext" fi if test "$GNULIB_ISBLANK" != 1; then if test "$GNULIB_ISBLANK" = 0; then GNULIB_ISBLANK=$gl_module_indicator_condition else GNULIB_ISBLANK="($GNULIB_ISBLANK || $gl_module_indicator_condition)" fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether isnan(double) can be used without linking with libm" >&5 $as_echo_n "checking whether isnan(double) can be used without linking with libm... " >&6; } if ${gl_cv_func_isnand_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNUC__ >= 4 # undef isnand # define isnand(x) __builtin_isnan ((double)(x)) #else # undef isnand # define isnand(x) isnan ((double)(x)) #endif double x; int main () { return isnand (x); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_isnand_no_libm=yes else gl_cv_func_isnand_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_isnand_no_libm" >&5 $as_echo "$gl_cv_func_isnand_no_libm" >&6; } gl_func_isnand_no_libm=$gl_cv_func_isnand_no_libm if test $gl_cv_func_isnand_no_libm = yes; then $as_echo "#define HAVE_ISNAND_IN_LIBC 1" >>confdefs.h fi if test $gl_func_isnand_no_libm != yes; then gltests_LIBOBJS="$gltests_LIBOBJS isnand.$ac_objext" fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'double'" >&5 $as_echo_n "checking where to find the exponent in a 'double'... " >&6; } if ${gl_cv_cc_double_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if defined arm || defined __arm || defined __arm__ mixed_endianness #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "mixed_endianness" >/dev/null 2>&1; then : gl_cv_cc_double_expbit0="unknown" else : if ${ac_cv_c_bigendian+:} false; then : $as_echo_n "(cached) " >&6 else ac_cv_c_bigendian=unknown # See if we're dealing with a universal compiler. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # Check for potential -arch flags. It is not universal unless # there are at least two -arch flags with different values. ac_arch= ac_prev= for ac_word in $CC $CFLAGS $CPPFLAGS $LDFLAGS; do if test -n "$ac_prev"; then case $ac_word in i?86 | x86_64 | ppc | ppc64) if test -z "$ac_arch" || test "$ac_arch" = "$ac_word"; then ac_arch=$ac_word else ac_cv_c_bigendian=universal break fi ;; esac ac_prev= elif test "x$ac_word" = "x-arch"; then ac_prev=arch fi done fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $ac_cv_c_bigendian = unknown; then # See if sys/param.h defines the BYTE_ORDER macro. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if ! (defined BYTE_ORDER && defined BIG_ENDIAN \ && defined LITTLE_ENDIAN && BYTE_ORDER && BIG_ENDIAN \ && LITTLE_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int main () { #if BYTE_ORDER != BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # See if defines _LITTLE_ENDIAN or _BIG_ENDIAN (e.g., Solaris). cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #if ! (defined _LITTLE_ENDIAN || defined _BIG_ENDIAN) bogus endian macros #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : # It does; now see whether it defined to _BIG_ENDIAN or not. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #ifndef _BIG_ENDIAN not big endian #endif ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_c_bigendian=yes else ac_cv_c_bigendian=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi if test $ac_cv_c_bigendian = unknown; then # Compile a test program. if test "$cross_compiling" = yes; then : # Try to guess by grepping values from an object file. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ short int ascii_mm[] = { 0x4249, 0x4765, 0x6E44, 0x6961, 0x6E53, 0x7953, 0 }; short int ascii_ii[] = { 0x694C, 0x5454, 0x656C, 0x6E45, 0x6944, 0x6E61, 0 }; int use_ascii (int i) { return ascii_mm[i] + ascii_ii[i]; } short int ebcdic_ii[] = { 0x89D3, 0xE3E3, 0x8593, 0x95C5, 0x89C4, 0x9581, 0 }; short int ebcdic_mm[] = { 0xC2C9, 0xC785, 0x95C4, 0x8981, 0x95E2, 0xA8E2, 0 }; int use_ebcdic (int i) { return ebcdic_mm[i] + ebcdic_ii[i]; } extern int foo; int main () { return use_ascii (foo) == use_ebcdic (foo); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : if grep BIGenDianSyS conftest.$ac_objext >/dev/null; then ac_cv_c_bigendian=yes fi if grep LiTTleEnDian conftest.$ac_objext >/dev/null ; then if test "$ac_cv_c_bigendian" = unknown; then ac_cv_c_bigendian=no else # finding both strings is unlikely to happen, but who knows? ac_cv_c_bigendian=unknown fi fi fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ $ac_includes_default int main () { /* Are we little or big endian? From Harbison&Steele. */ union { long int l; char c[sizeof (long int)]; } u; u.l = 1; return u.c[sizeof (long int) - 1] == 1; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : ac_cv_c_bigendian=no else ac_cv_c_bigendian=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi : case $ac_cv_c_bigendian in #( yes) gl_cv_cc_double_expbit0="word 0 bit 20";; #( no) gl_cv_cc_double_expbit0="word 1 bit 20" ;; #( universal) $as_echo "#define AC_APPLE_UNIVERSAL_BUILD 1" >>confdefs.h ;; #( *) gl_cv_cc_double_expbit0="unknown" ;; esac fi rm -f conftest* else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (double x) { memory_double m; size_t i; /* Clear it first, in case sizeof (double) < sizeof (memory_double). */ memset (&m, 0, sizeof (memory_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25); add_to_ored_words (0.5); add_to_ored_words (1.0); add_to_ored_words (2.0); add_to_ored_words (4.0); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_double_expbit0=`cat conftest.out` else gl_cv_cc_double_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_double_expbit0" >&5 $as_echo "$gl_cv_cc_double_expbit0" >&6; } case "$gl_cv_cc_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define DBL_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define DBL_EXPBIT0_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether isnan(float) can be used without linking with libm" >&5 $as_echo_n "checking whether isnan(float) can be used without linking with libm... " >&6; } if ${gl_cv_func_isnanf_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNUC__ >= 4 # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) #elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) #endif float x; int main () { return isnanf (x); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_isnanf_no_libm=yes else gl_cv_func_isnanf_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_isnanf_no_libm" >&5 $as_echo "$gl_cv_func_isnanf_no_libm" >&6; } if test $gl_cv_func_isnanf_no_libm = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether isnan(float) works" >&5 $as_echo_n "checking whether isnan(float) works... " >&6; } if ${gl_cv_func_isnanf_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in irix* | solaris*) gl_cv_func_isnanf_works="guessing no" ;; mingw*) # Guess yes on mingw, no on MSVC. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __MINGW32__ Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_func_isnanf_works="guessing yes" else gl_cv_func_isnanf_works="guessing no" fi rm -f conftest* ;; *) gl_cv_func_isnanf_works="guessing yes" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNUC__ >= 4 # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) #elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) #endif /* The Compaq (ex-DEC) C 6.4 compiler chokes on the expression 0.0 / 0.0. */ #ifdef __DECC static float NaN () { static float zero = 0.0f; return zero / zero; } #else # define NaN() (0.0f / 0.0f) #endif #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { unsigned int word[NWORDS]; float value; } memory_float; int main() { int result = 0; if (isnanf (1.0f / 0.0f)) result |= 1; if (!isnanf (NaN ())) result |= 2; #if defined FLT_EXPBIT0_WORD && defined FLT_EXPBIT0_BIT /* The isnanf function should be immune against changes in the sign bit and in the mantissa bits. The xor operation twiddles a bit that can only be a sign bit or a mantissa bit. */ if (FLT_EXPBIT0_WORD == 0 && FLT_EXPBIT0_BIT > 0) { memory_float m; m.value = NaN (); /* Set the bits below the exponent to 01111...111. */ m.word[0] &= -1U << FLT_EXPBIT0_BIT; m.word[0] |= 1U << (FLT_EXPBIT0_BIT - 1) - 1; if (!isnanf (m.value)) result |= 4; } #endif return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_isnanf_works=yes else gl_cv_func_isnanf_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_isnanf_works" >&5 $as_echo "$gl_cv_func_isnanf_works" >&6; } fi if test $gl_cv_func_isnanf_no_libm = yes \ && { case "$gl_cv_func_isnanf_works" in *yes) true;; *) false;; esac }; then gl_func_isnanf_no_libm=yes $as_echo "#define HAVE_ISNANF_IN_LIBC 1" >>confdefs.h else gl_func_isnanf_no_libm=no fi if test $gl_func_isnanf_no_libm != yes; then gltests_LIBOBJS="$gltests_LIBOBJS isnanf.$ac_objext" { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'float'" >&5 $as_echo_n "checking where to find the exponent in a 'float'... " >&6; } if ${gl_cv_cc_float_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_float_expbit0="word 0 bit 23" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (float x) { memory_float m; size_t i; /* Clear it first, in case sizeof (float) < sizeof (memory_float). */ memset (&m, 0, sizeof (memory_float)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25f); add_to_ored_words (0.5f); add_to_ored_words (1.0f); add_to_ored_words (2.0f); add_to_ored_words (4.0f); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_float_expbit0=`cat conftest.out` else gl_cv_cc_float_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_float_expbit0" >&5 $as_echo "$gl_cv_cc_float_expbit0" >&6; } case "$gl_cv_cc_float_expbit0" in word*bit*) word=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define FLT_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define FLT_EXPBIT0_BIT $bit _ACEOF ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'float'" >&5 $as_echo_n "checking where to find the exponent in a 'float'... " >&6; } if ${gl_cv_cc_float_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_float_expbit0="word 0 bit 23" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (float x) { memory_float m; size_t i; /* Clear it first, in case sizeof (float) < sizeof (memory_float). */ memset (&m, 0, sizeof (memory_float)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25f); add_to_ored_words (0.5f); add_to_ored_words (1.0f); add_to_ored_words (2.0f); add_to_ored_words (4.0f); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_float_expbit0=`cat conftest.out` else gl_cv_cc_float_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_float_expbit0" >&5 $as_echo "$gl_cv_cc_float_expbit0" >&6; } case "$gl_cv_cc_float_expbit0" in word*bit*) word=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define FLT_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define FLT_EXPBIT0_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether isnan(long double) can be used without linking with libm" >&5 $as_echo_n "checking whether isnan(long double) can be used without linking with libm... " >&6; } if ${gl_cv_func_isnanl_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #if __GNUC__ >= 4 # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) #elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) #endif long double x; int main () { return isnanl (x); ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_isnanl_no_libm=yes else gl_cv_func_isnanl_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_isnanl_no_libm" >&5 $as_echo "$gl_cv_func_isnanl_no_libm" >&6; } gl_func_isnanl_no_libm=$gl_cv_func_isnanl_no_libm if test $gl_func_isnanl_no_libm = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether isnanl works" >&5 $as_echo_n "checking whether isnanl works... " >&6; } if ${gl_cv_func_isnanl_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in mingw*) # Guess yes on mingw, no on MSVC. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __MINGW32__ Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_func_isnanl_works="guessing yes" else gl_cv_func_isnanl_works="guessing no" fi rm -f conftest* ;; *) gl_cv_func_isnanl_works="guessing yes" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if __GNUC__ >= 4 # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) #elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) #endif #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { unsigned int word[NWORDS]; long double value; } memory_long_double; /* On Irix 6.5, gcc 3.4.3 can't compute compile-time NaN, and needs the runtime type conversion. */ #ifdef __sgi static long double NaNl () { double zero = 0.0; return zero / zero; } #else # define NaNl() (0.0L / 0.0L) #endif int main () { int result = 0; if (!isnanl (NaNl ())) result |= 1; { memory_long_double m; unsigned int i; /* The isnanl function should be immune against changes in the sign bit and in the mantissa bits. The xor operation twiddles a bit that can only be a sign bit or a mantissa bit (since the exponent never extends to bit 31). */ m.value = NaNl (); m.word[NWORDS / 2] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); for (i = 0; i < NWORDS; i++) m.word[i] |= 1; if (!isnanl (m.value)) result |= 1; } #if ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Representation of an 80-bit 'long double' as an initializer for a sequence of 'unsigned int' words. */ # ifdef WORDS_BIGENDIAN # define LDBL80_WORDS(exponent,manthi,mantlo) \ { ((unsigned int) (exponent) << 16) | ((unsigned int) (manthi) >> 16), \ ((unsigned int) (manthi) << 16) | ((unsigned int) (mantlo) >> 16), \ (unsigned int) (mantlo) << 16 \ } # else # define LDBL80_WORDS(exponent,manthi,mantlo) \ { mantlo, manthi, exponent } # endif { /* Quiet NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0xC3333333, 0x00000000) }; if (!isnanl (x.value)) result |= 2; } { /* Signalling NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x83333333, 0x00000000) }; if (!isnanl (x.value)) result |= 2; } /* isnanl should return something even for noncanonical values. */ { /* Pseudo-NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x40000001, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 4; } { /* Pseudo-Infinity. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x00000000, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 8; } { /* Pseudo-Zero. */ static memory_long_double x = { LDBL80_WORDS (0x4004, 0x00000000, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 16; } { /* Unnormalized number. */ static memory_long_double x = { LDBL80_WORDS (0x4000, 0x63333333, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 32; } { /* Pseudo-Denormal. */ static memory_long_double x = { LDBL80_WORDS (0x0000, 0x83333333, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 64; } #endif return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_isnanl_works=yes else gl_cv_func_isnanl_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_isnanl_works" >&5 $as_echo "$gl_cv_func_isnanl_works" >&6; } case "$gl_cv_func_isnanl_works" in *yes) ;; *) gl_func_isnanl_no_libm=no ;; esac fi if test $gl_func_isnanl_no_libm = yes; then $as_echo "#define HAVE_ISNANL_IN_LIBC 1" >>confdefs.h fi if test $gl_func_isnanl_no_libm != yes; then gltests_LIBOBJS="$gltests_LIBOBJS isnanl.$ac_objext" { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'long double'" >&5 $as_echo_n "checking where to find the exponent in a 'long double'... " >&6; } if ${gl_cv_cc_long_double_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_long_double_expbit0="unknown" case "$host_os" in mingw*) # On native Windows (little-endian), we know the result # in two cases: mingw, MSVC. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __MINGW32__ Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_cc_long_double_expbit0="word 2 bit 0" fi rm -f conftest* cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef _MSC_VER Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_cc_long_double_expbit0="word 1 bit 20" fi rm -f conftest* ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { long double value; unsigned int word[NWORDS]; } memory_long_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (long double x) { memory_long_double m; size_t i; /* Clear it first, in case sizeof (long double) < sizeof (memory_long_double). */ memset (&m, 0, sizeof (memory_long_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25L); add_to_ored_words (0.5L); add_to_ored_words (1.0L); add_to_ored_words (2.0L); add_to_ored_words (4.0L); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_long_double_expbit0=`cat conftest.out` else gl_cv_cc_long_double_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_long_double_expbit0" >&5 $as_echo "$gl_cv_cc_long_double_expbit0" >&6; } case "$gl_cv_cc_long_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_long_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_long_double_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define LDBL_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define LDBL_EXPBIT0_BIT $bit _ACEOF ;; esac fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the exponent in a 'long double'" >&5 $as_echo_n "checking where to find the exponent in a 'long double'... " >&6; } if ${gl_cv_cc_long_double_expbit0+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_long_double_expbit0="unknown" case "$host_os" in mingw*) # On native Windows (little-endian), we know the result # in two cases: mingw, MSVC. cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef __MINGW32__ Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_cc_long_double_expbit0="word 2 bit 0" fi rm -f conftest* cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #ifdef _MSC_VER Known #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "Known" >/dev/null 2>&1; then : gl_cv_cc_long_double_expbit0="word 1 bit 20" fi rm -f conftest* ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #include #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { long double value; unsigned int word[NWORDS]; } memory_long_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (long double x) { memory_long_double m; size_t i; /* Clear it first, in case sizeof (long double) < sizeof (memory_long_double). */ memset (&m, 0, sizeof (memory_long_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25L); add_to_ored_words (0.5L); add_to_ored_words (1.0L); add_to_ored_words (2.0L); add_to_ored_words (4.0L); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_long_double_expbit0=`cat conftest.out` else gl_cv_cc_long_double_expbit0="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_long_double_expbit0" >&5 $as_echo "$gl_cv_cc_long_double_expbit0" >&6; } case "$gl_cv_cc_long_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_long_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_long_double_expbit0" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define LDBL_EXPBIT0_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define LDBL_EXPBIT0_BIT $bit _ACEOF ;; esac if test "$ac_cv_header_winsock2_h" = yes; then gltests_LIBOBJS="$gltests_LIBOBJS listen.$ac_objext" fi if test "$GNULIB_LISTEN" != 1; then if test "$GNULIB_LISTEN" = 0; then GNULIB_LISTEN=$gl_module_indicator_condition else GNULIB_LISTEN="($GNULIB_LISTEN || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_LISTEN 1" >>confdefs.h for ac_func in setlocale uselocale do : as_ac_var=`$as_echo "ac_cv_func_$ac_func" | $as_tr_sh` ac_fn_c_check_func "$LINENO" "$ac_func" "$as_ac_var" if eval test \"x\$"$as_ac_var"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done if test $ac_cv_func_uselocale = yes; then for ac_func in getlocalename_l do : ac_fn_c_check_func "$LINENO" "getlocalename_l" "ac_cv_func_getlocalename_l" if test "x$ac_cv_func_getlocalename_l" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_GETLOCALENAME_L 1 _ACEOF fi done fi gltests_LIBOBJS="$gltests_LIBOBJS localtime-buffer.$ac_objext" if test $ac_cv_func_lstat = yes; then case $host_os,$gl_cv_func_lstat_dereferences_slashed_symlink in solaris* | *no) REPLACE_LSTAT=1 ;; esac else HAVE_LSTAT=0 fi if test $REPLACE_LSTAT = 1; then gltests_LIBOBJS="$gltests_LIBOBJS lstat.$ac_objext" : fi if test "$GNULIB_LSTAT" != 1; then if test "$GNULIB_LSTAT" = 0; then GNULIB_LSTAT=$gl_module_indicator_condition else GNULIB_LSTAT="($GNULIB_LSTAT || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_LSTAT 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional french locale" >&5 $as_echo_n "checking for a traditional french locale... " >&6; } if ${gt_cv_locale_fr+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; # if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; # endif return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... 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Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 # Check for mmap(). Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. ac_fn_c_check_func "$LINENO" "mmap" "ac_cv_func_mmap" if test "x$ac_cv_func_mmap" = xyes; then : gl_have_mmap=yes else gl_have_mmap=no fi # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for MAP_ANONYMOUS" >&5 $as_echo_n "checking for MAP_ANONYMOUS... 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LIB_NANOSLEEP= { $as_echo "$as_me:${as_lineno-$LINENO}: checking for library containing nanosleep" >&5 $as_echo_n "checking for library containing nanosleep... " >&6; } if ${ac_cv_search_nanosleep+:} false; then : $as_echo_n "(cached) " >&6 else ac_func_search_save_LIBS=$LIBS cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char nanosleep (); int main () { return nanosleep (); ; return 0; } _ACEOF for ac_lib in '' rt posix4; do if test -z "$ac_lib"; then ac_res="none required" else ac_res=-l$ac_lib LIBS="-l$ac_lib $ac_func_search_save_LIBS" fi if ac_fn_c_try_link "$LINENO"; then : ac_cv_search_nanosleep=$ac_res fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext if ${ac_cv_search_nanosleep+:} false; then : break fi done if ${ac_cv_search_nanosleep+:} false; then : else ac_cv_search_nanosleep=no fi rm conftest.$ac_ext LIBS=$ac_func_search_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_search_nanosleep" >&5 $as_echo "$ac_cv_search_nanosleep" >&6; } ac_res=$ac_cv_search_nanosleep if test "$ac_res" != no; then : test "$ac_res" = "none required" || LIBS="$ac_res $LIBS" test "$ac_cv_search_nanosleep" = "none required" || LIB_NANOSLEEP=$ac_cv_search_nanosleep fi if test "x$ac_cv_search_nanosleep" != xno; then if test $APPLE_UNIVERSAL_BUILD = 1; then # A universal build on Apple Mac OS X platforms. # The test result would be 'no (mishandles large arguments)' in 64-bit # mode but 'yes' in 32-bit mode. But we need a configuration result that # is valid in both modes. gl_cv_func_nanosleep='no (mishandles large arguments)' fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking for working nanosleep" >&5 $as_echo_n "checking for working nanosleep... " >&6; } if ${gl_cv_func_nanosleep+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in linux*) # Guess it halfway works when the kernel is Linux. gl_cv_func_nanosleep='guessing no (mishandles large arguments)' ;; mingw*) # Guess no on native Windows. gl_cv_func_nanosleep='guessing no' ;; *) # If we don't know, assume the worst. gl_cv_func_nanosleep='guessing no' ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_SYS_TIME_H #include #endif #include #include #define TYPE_SIGNED(t) (! ((t) 0 < (t) -1)) #define TYPE_MAXIMUM(t) \ ((t) (! TYPE_SIGNED (t) \ ? (t) -1 \ : ((((t) 1 << (sizeof (t) * CHAR_BIT - 2)) - 1) * 2 + 1))) static void check_for_SIGALRM (int sig) { if (sig != SIGALRM) _exit (1); } int main () { static struct timespec ts_sleep; static struct timespec ts_remaining; static struct sigaction act; /* Test for major problems first. */ if (! nanosleep) return 2; act.sa_handler = check_for_SIGALRM; sigemptyset (&act.sa_mask); sigaction (SIGALRM, &act, NULL); ts_sleep.tv_sec = 0; ts_sleep.tv_nsec = 1; alarm (1); if (nanosleep (&ts_sleep, NULL) != 0) return 3; /* Test for a minor problem: the handling of large arguments. */ ts_sleep.tv_sec = TYPE_MAXIMUM (time_t); ts_sleep.tv_nsec = 999999999; alarm (1); if (nanosleep (&ts_sleep, &ts_remaining) != -1) return 4; if (errno != EINTR) return 5; if (ts_remaining.tv_sec <= TYPE_MAXIMUM (time_t) - 10) return 6; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_nanosleep=yes else case $? in 4|5|6) gl_cv_func_nanosleep='no (mishandles large arguments)';; *) gl_cv_func_nanosleep=no;; esac fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_nanosleep" >&5 $as_echo "$gl_cv_func_nanosleep" >&6; } case "$gl_cv_func_nanosleep" in *yes) REPLACE_NANOSLEEP=0 ;; *) REPLACE_NANOSLEEP=1 case "$gl_cv_func_nanosleep" in *"mishandles large arguments"*) $as_echo "#define HAVE_BUG_BIG_NANOSLEEP 1" >>confdefs.h ;; *) # The replacement uses select(). Add $LIBSOCKET to $LIB_NANOSLEEP. for ac_lib in $LIBSOCKET; do case " $LIB_NANOSLEEP " in *" $ac_lib "*) ;; *) LIB_NANOSLEEP="$LIB_NANOSLEEP $ac_lib";; esac done ;; esac ;; esac else HAVE_NANOSLEEP=0 fi LIBS=$nanosleep_save_libs if test $HAVE_NANOSLEEP = 0 || test $REPLACE_NANOSLEEP = 1; then gltests_LIBOBJS="$gltests_LIBOBJS nanosleep.$ac_objext" : fi if test "$GNULIB_NANOSLEEP" != 1; then if test "$GNULIB_NANOSLEEP" = 0; then GNULIB_NANOSLEEP=$gl_module_indicator_condition else GNULIB_NANOSLEEP="($GNULIB_NANOSLEEP || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_NANOSLEEP 1" >>confdefs.h { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether is self-contained" >&5 $as_echo_n "checking whether is self-contained... 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Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. ac_fn_c_check_func "$LINENO" "mmap" "ac_cv_func_mmap" if test "x$ac_cv_func_mmap" = xyes; then : gl_have_mmap=yes else gl_have_mmap=no fi # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for MAP_ANONYMOUS" >&5 $as_echo_n "checking for MAP_ANONYMOUS... 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Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... 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Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_zh_CN" >&5 $as_echo "$gt_cv_locale_zh_CN" >&6; } LOCALE_ZH_CN=$gt_cv_locale_zh_CN if test "$ac_cv_header_winsock2_h" = yes; then gltests_LIBOBJS="$gltests_LIBOBJS setsockopt.$ac_objext" fi if test "$GNULIB_SETSOCKOPT" != 1; then if test "$GNULIB_SETSOCKOPT" = 0; then GNULIB_SETSOCKOPT=$gl_module_indicator_condition else GNULIB_SETSOCKOPT="($GNULIB_SETSOCKOPT || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SETSOCKOPT 1" >>confdefs.h if test $ac_cv_func_sigaction = yes; then ac_fn_c_check_member "$LINENO" "struct sigaction" "sa_sigaction" "ac_cv_member_struct_sigaction_sa_sigaction" "#include " if test "x$ac_cv_member_struct_sigaction_sa_sigaction" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_SIGACTION_SA_SIGACTION 1 _ACEOF fi if test $ac_cv_member_struct_sigaction_sa_sigaction = no; then HAVE_STRUCT_SIGACTION_SA_SIGACTION=0 fi else HAVE_SIGACTION=0 fi if test $HAVE_SIGACTION = 0; then gltests_LIBOBJS="$gltests_LIBOBJS sigaction.$ac_objext" ac_fn_c_check_type "$LINENO" "siginfo_t" "ac_cv_type_siginfo_t" " #include " if test "x$ac_cv_type_siginfo_t" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_SIGINFO_T 1 _ACEOF fi if test $ac_cv_type_siginfo_t = no; then HAVE_SIGINFO_T=0 fi fi if test "$GNULIB_SIGACTION" != 1; then if test "$GNULIB_SIGACTION" = 0; then GNULIB_SIGACTION=$gl_module_indicator_condition else GNULIB_SIGACTION="($GNULIB_SIGACTION || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SIGACTION 1" >>confdefs.h if test $gl_cv_have_include_next = yes; then gl_cv_next_signal_h='<'signal.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_signal_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'signal.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_signal_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_signal_h gl_cv_next_signal_h='"'$gl_header'"' fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_signal_h" >&5 $as_echo "$gl_cv_next_signal_h" >&6; } fi NEXT_SIGNAL_H=$gl_cv_next_signal_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'signal.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_signal_h fi NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H=$gl_next_as_first_directive # AIX declares sig_atomic_t to already include volatile, and C89 compilers # then choke on 'volatile sig_atomic_t'. C99 requires that it compile. ac_fn_c_check_type "$LINENO" "volatile sig_atomic_t" "ac_cv_type_volatile_sig_atomic_t" " #include " if test "x$ac_cv_type_volatile_sig_atomic_t" = xyes; then : else HAVE_TYPE_VOLATILE_SIG_ATOMIC_T=0 fi ac_fn_c_check_type "$LINENO" "sighandler_t" "ac_cv_type_sighandler_t" " #include " if test "x$ac_cv_type_sighandler_t" = xyes; then : else HAVE_SIGHANDLER_T=0 fi for gl_func in pthread_sigmask sigaction sigaddset sigdelset sigemptyset sigfillset sigismember sigpending sigprocmask; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done { $as_echo "$as_me:${as_lineno-$LINENO}: checking for signbit macro" >&5 $as_echo_n "checking for signbit macro... 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Needed because GCC 4 constant-folds __builtin_signbitl (literal) but cannot constant-fold __builtin_signbitl (variable). */ float vf; double vd; long double vl; int main () { /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0. So we use -p0f and -p0d instead. */ float p0f = 0.0f; float m0f = -p0f; double p0d = 0.0; double m0d = -p0d; /* On HP-UX 10.20, negating 0.0L does not yield -0.0L. So we use another constant expression instead. But that expression does not work on other platforms, such as when cross-compiling to PowerPC on Mac OS X 10.5. */ long double p0l = 0.0L; #if defined __hpux || defined __sgi long double m0l = -LDBL_MIN * LDBL_MIN; #else long double m0l = -p0l; #endif int result = 0; if (signbit (vf)) /* link check */ vf++; { float plus_inf = 1.0f / p0f; float minus_inf = -1.0f / p0f; if (!(!signbit (255.0f) && signbit (-255.0f) && !signbit (p0f) && (memcmp (&m0f, &p0f, sizeof (float)) == 0 || signbit (m0f)) && !signbit (plus_inf) && signbit (minus_inf))) result |= 1; } if (signbit (vd)) /* link check */ vd++; { double plus_inf = 1.0 / p0d; double minus_inf = -1.0 / p0d; if (!(!signbit (255.0) && signbit (-255.0) && !signbit (p0d) && (memcmp (&m0d, &p0d, sizeof (double)) == 0 || signbit (m0d)) && !signbit (plus_inf) && signbit (minus_inf))) result |= 2; } if (signbit (vl)) /* link check */ vl++; { long double plus_inf = 1.0L / p0l; long double minus_inf = -1.0L / p0l; if (signbit (255.0L)) result |= 4; if (!signbit (-255.0L)) result |= 4; if (signbit (p0l)) result |= 8; if (!(memcmp (&m0l, &p0l, sizeof (long double)) == 0 || signbit (m0l))) result |= 16; if (signbit (plus_inf)) result |= 32; if (!signbit (minus_inf)) result |= 64; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_signbit=yes else gl_cv_func_signbit=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_signbit" >&5 $as_echo "$gl_cv_func_signbit" >&6; } { $as_echo "$as_me:${as_lineno-$LINENO}: checking for signbit compiler built-ins" >&5 $as_echo_n "checking for signbit compiler built-ins... " >&6; } if ${gl_cv_func_signbit_gcc+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_signbit_gcc="guessing yes" ;; # Guess yes on mingw, no on MSVC. mingw*) if test -n "$GCC"; then gl_cv_func_signbit_gcc="guessing yes" else gl_cv_func_signbit_gcc="guessing no" fi ;; # If we don't know, assume the worst. *) gl_cv_func_signbit_gcc="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #if __GNUC__ >= 4 # define signbit(x) \ (sizeof (x) == sizeof (long double) ? __builtin_signbitl (x) : \ sizeof (x) == sizeof (double) ? __builtin_signbit (x) : \ __builtin_signbitf (x)) #else # error "signbit should be three compiler built-ins" #endif #include /* Global variables. Needed because GCC 4 constant-folds __builtin_signbitl (literal) but cannot constant-fold __builtin_signbitl (variable). */ float vf; double vd; long double vl; int main () { /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0. So we use -p0f and -p0d instead. */ float p0f = 0.0f; float m0f = -p0f; double p0d = 0.0; double m0d = -p0d; /* On HP-UX 10.20, negating 0.0L does not yield -0.0L. So we use another constant expression instead. But that expression does not work on other platforms, such as when cross-compiling to PowerPC on Mac OS X 10.5. */ long double p0l = 0.0L; #if defined __hpux || defined __sgi long double m0l = -LDBL_MIN * LDBL_MIN; #else long double m0l = -p0l; #endif int result = 0; if (signbit (vf)) /* link check */ vf++; { float plus_inf = 1.0f / p0f; float minus_inf = -1.0f / p0f; if (!(!signbit (255.0f) && signbit (-255.0f) && !signbit (p0f) && (memcmp (&m0f, &p0f, sizeof (float)) == 0 || signbit (m0f)) && !signbit (plus_inf) && signbit (minus_inf))) result |= 1; } if (signbit (vd)) /* link check */ vd++; { double plus_inf = 1.0 / p0d; double minus_inf = -1.0 / p0d; if (!(!signbit (255.0) && signbit (-255.0) && !signbit (p0d) && (memcmp (&m0d, &p0d, sizeof (double)) == 0 || signbit (m0d)) && !signbit (plus_inf) && signbit (minus_inf))) result |= 2; } if (signbit (vl)) /* link check */ vl++; { long double plus_inf = 1.0L / p0l; long double minus_inf = -1.0L / p0l; if (signbit (255.0L)) result |= 4; if (!signbit (-255.0L)) result |= 4; if (signbit (p0l)) result |= 8; if (!(memcmp (&m0l, &p0l, sizeof (long double)) == 0 || signbit (m0l))) result |= 16; if (signbit (plus_inf)) result |= 32; if (!signbit (minus_inf)) result |= 64; } return result; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_signbit_gcc=yes else gl_cv_func_signbit_gcc=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_signbit_gcc" >&5 $as_echo "$gl_cv_func_signbit_gcc" >&6; } case "$gl_cv_func_signbit_gcc" in *yes) REPLACE_SIGNBIT_USING_GCC=1 ;; *) case "$gl_cv_func_signbit" in *yes) ;; *) REPLACE_SIGNBIT=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the sign bit in a 'float'" >&5 $as_echo_n "checking where to find the sign bit in a 'float'... " >&6; } if ${gl_cv_cc_float_signbit+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_float_signbit="unknown" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; static memory_float plus = { 1.0f }; static memory_float minus = { -1.0f }; int main () { size_t j, k, i; unsigned int m; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; /* Find the different bit. */ k = 0; m = 0; for (j = 0; j < NWORDS; j++) { unsigned int x = plus.word[j] ^ minus.word[j]; if ((x & (x - 1)) || (x && m)) { /* More than one bit difference. */ fprintf (fp, "unknown"); fclose (fp); return 2; } if (x) { k = j; m = x; } } if (m == 0) { /* No difference. */ fprintf (fp, "unknown"); fclose (fp); return 3; } /* Now m = plus.word[k] ^ ~minus.word[k]. */ if (plus.word[k] & ~minus.word[k]) { /* Oh? The sign bit is set in the positive and cleared in the negative numbers? */ fprintf (fp, "unknown"); fclose (fp); return 4; } for (i = 0; ; i++) if ((m >> i) & 1) break; fprintf (fp, "word %d bit %d", (int) k, (int) i); if (fclose (fp) != 0) return 5; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_float_signbit=`cat conftest.out` else gl_cv_cc_float_signbit="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_float_signbit" >&5 $as_echo "$gl_cv_cc_float_signbit" >&6; } case "$gl_cv_cc_float_signbit" in word*bit*) word=`echo "$gl_cv_cc_float_signbit" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_float_signbit" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define FLT_SIGNBIT_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define FLT_SIGNBIT_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the sign bit in a 'double'" >&5 $as_echo_n "checking where to find the sign bit in a 'double'... " >&6; } if ${gl_cv_cc_double_signbit+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_double_signbit="unknown" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_float; static memory_float plus = { 1.0 }; static memory_float minus = { -1.0 }; int main () { size_t j, k, i; unsigned int m; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; /* Find the different bit. */ k = 0; m = 0; for (j = 0; j < NWORDS; j++) { unsigned int x = plus.word[j] ^ minus.word[j]; if ((x & (x - 1)) || (x && m)) { /* More than one bit difference. */ fprintf (fp, "unknown"); fclose (fp); return 2; } if (x) { k = j; m = x; } } if (m == 0) { /* No difference. */ fprintf (fp, "unknown"); fclose (fp); return 3; } /* Now m = plus.word[k] ^ ~minus.word[k]. */ if (plus.word[k] & ~minus.word[k]) { /* Oh? The sign bit is set in the positive and cleared in the negative numbers? */ fprintf (fp, "unknown"); fclose (fp); return 4; } for (i = 0; ; i++) if ((m >> i) & 1) break; fprintf (fp, "word %d bit %d", (int) k, (int) i); if (fclose (fp) != 0) return 5; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_double_signbit=`cat conftest.out` else gl_cv_cc_double_signbit="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_double_signbit" >&5 $as_echo "$gl_cv_cc_double_signbit" >&6; } case "$gl_cv_cc_double_signbit" in word*bit*) word=`echo "$gl_cv_cc_double_signbit" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_double_signbit" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define DBL_SIGNBIT_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define DBL_SIGNBIT_BIT $bit _ACEOF ;; esac { $as_echo "$as_me:${as_lineno-$LINENO}: checking where to find the sign bit in a 'long double'" >&5 $as_echo_n "checking where to find the sign bit in a 'long double'... " >&6; } if ${gl_cv_cc_long_double_signbit+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : gl_cv_cc_long_double_signbit="unknown" else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { long double value; unsigned int word[NWORDS]; } memory_float; static memory_float plus = { 1.0L }; static memory_float minus = { -1.0L }; int main () { size_t j, k, i; unsigned int m; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; /* Find the different bit. */ k = 0; m = 0; for (j = 0; j < NWORDS; j++) { unsigned int x = plus.word[j] ^ minus.word[j]; if ((x & (x - 1)) || (x && m)) { /* More than one bit difference. */ fprintf (fp, "unknown"); fclose (fp); return 2; } if (x) { k = j; m = x; } } if (m == 0) { /* No difference. */ fprintf (fp, "unknown"); fclose (fp); return 3; } /* Now m = plus.word[k] ^ ~minus.word[k]. */ if (plus.word[k] & ~minus.word[k]) { /* Oh? The sign bit is set in the positive and cleared in the negative numbers? */ fprintf (fp, "unknown"); fclose (fp); return 4; } for (i = 0; ; i++) if ((m >> i) & 1) break; fprintf (fp, "word %d bit %d", (int) k, (int) i); if (fclose (fp) != 0) return 5; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_cc_long_double_signbit=`cat conftest.out` else gl_cv_cc_long_double_signbit="unknown" fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.out fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_cc_long_double_signbit" >&5 $as_echo "$gl_cv_cc_long_double_signbit" >&6; } case "$gl_cv_cc_long_double_signbit" in word*bit*) word=`echo "$gl_cv_cc_long_double_signbit" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_long_double_signbit" | sed -e 's/word.*bit //'` cat >>confdefs.h <<_ACEOF #define LDBL_SIGNBIT_WORD $word _ACEOF cat >>confdefs.h <<_ACEOF #define LDBL_SIGNBIT_BIT $bit _ACEOF ;; esac if test "$gl_cv_cc_float_signbit" = unknown; then ac_fn_c_check_decl "$LINENO" "copysignf" "ac_cv_have_decl_copysignf" "#include " if test "x$ac_cv_have_decl_copysignf" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_COPYSIGNF $ac_have_decl _ACEOF if test "$ac_cv_have_decl_copysignf" = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether copysignf can be used without linking with libm" >&5 $as_echo_n "checking whether copysignf can be used without linking with libm... " >&6; } if ${gl_cv_func_copysignf_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include float x, y; int main () { return copysignf (x, y) < 0; ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_copysignf_no_libm=yes else gl_cv_func_copysignf_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_copysignf_no_libm" >&5 $as_echo "$gl_cv_func_copysignf_no_libm" >&6; } if test $gl_cv_func_copysignf_no_libm = yes; then $as_echo "#define HAVE_COPYSIGNF_IN_LIBC 1" >>confdefs.h fi fi fi if test "$gl_cv_cc_double_signbit" = unknown; then ac_fn_c_check_decl "$LINENO" "copysign" "ac_cv_have_decl_copysign" "#include " if test "x$ac_cv_have_decl_copysign" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_COPYSIGN $ac_have_decl _ACEOF if test "$ac_cv_have_decl_copysign" = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether copysign can be used without linking with libm" >&5 $as_echo_n "checking whether copysign can be used without linking with libm... " >&6; } if ${gl_cv_func_copysign_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include double x, y; int main () { return copysign (x, y) < 0; ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_copysign_no_libm=yes else gl_cv_func_copysign_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_copysign_no_libm" >&5 $as_echo "$gl_cv_func_copysign_no_libm" >&6; } if test $gl_cv_func_copysign_no_libm = yes; then $as_echo "#define HAVE_COPYSIGN_IN_LIBC 1" >>confdefs.h fi fi fi if test "$gl_cv_cc_long_double_signbit" = unknown; then ac_fn_c_check_decl "$LINENO" "copysignl" "ac_cv_have_decl_copysignl" "#include " if test "x$ac_cv_have_decl_copysignl" = xyes; then : ac_have_decl=1 else ac_have_decl=0 fi cat >>confdefs.h <<_ACEOF #define HAVE_DECL_COPYSIGNL $ac_have_decl _ACEOF if test "$ac_cv_have_decl_copysignl" = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether copysignl can be used without linking with libm" >&5 $as_echo_n "checking whether copysignl can be used without linking with libm... " >&6; } if ${gl_cv_func_copysignl_no_libm+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include long double x, y; int main () { return copysignl (x, y) < 0; ; return 0; } _ACEOF if ac_fn_c_try_link "$LINENO"; then : gl_cv_func_copysignl_no_libm=yes else gl_cv_func_copysignl_no_libm=no fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_copysignl_no_libm" >&5 $as_echo "$gl_cv_func_copysignl_no_libm" >&6; } if test $gl_cv_func_copysignl_no_libm = yes; then $as_echo "#define HAVE_COPYSIGNL_IN_LIBC 1" >>confdefs.h fi fi fi ;; esac ;; esac if test $REPLACE_SIGNBIT = 1; then gltests_LIBOBJS="$gltests_LIBOBJS signbitf.$ac_objext" gltests_LIBOBJS="$gltests_LIBOBJS signbitd.$ac_objext" gltests_LIBOBJS="$gltests_LIBOBJS signbitl.$ac_objext" fi if test "$GNULIB_SIGNBIT" != 1; then if test "$GNULIB_SIGNBIT" = 0; then GNULIB_SIGNBIT=$gl_module_indicator_condition else GNULIB_SIGNBIT="($GNULIB_SIGNBIT || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SIGNBIT 1" >>confdefs.h if test $gl_cv_type_sigset_t = yes; then ac_fn_c_check_func "$LINENO" "sigprocmask" "ac_cv_func_sigprocmask" if test "x$ac_cv_func_sigprocmask" = xyes; then : gl_cv_func_sigprocmask=1 fi fi if test -z "$gl_cv_func_sigprocmask"; then HAVE_POSIX_SIGNALBLOCKING=0 fi if test $HAVE_POSIX_SIGNALBLOCKING = 0; then gltests_LIBOBJS="$gltests_LIBOBJS sigprocmask.$ac_objext" : fi if test "$GNULIB_SIGPROCMASK" != 1; then if test "$GNULIB_SIGPROCMASK" = 0; then GNULIB_SIGPROCMASK=$gl_module_indicator_condition else GNULIB_SIGPROCMASK="($GNULIB_SIGPROCMASK || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SIGPROCMASK 1" >>confdefs.h if test "$ac_cv_header_winsock2_h" = yes; then gltests_LIBOBJS="$gltests_LIBOBJS socket.$ac_objext" fi # When this module is used, sockets may actually occur as file descriptors, # hence it is worth warning if the modules 'close' and 'ioctl' are not used. if test "$ac_cv_header_winsock2_h" = yes; then UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=1 SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=1 fi if test "$GNULIB_SOCKET" != 1; then if test "$GNULIB_SOCKET" = 0; then GNULIB_SOCKET=$gl_module_indicator_condition else GNULIB_SOCKET="($GNULIB_SOCKET || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SOCKET 1" >>confdefs.h ac_fn_c_check_type "$LINENO" "socklen_t" "ac_cv_type_socklen_t" " /* is not needed according to POSIX, but the in i386-unknown-freebsd4.10 and powerpc-apple-darwin5.5 required it. */ #include #if HAVE_SYS_SOCKET_H # include #elif HAVE_WS2TCPIP_H # include #endif " if test "x$ac_cv_type_socklen_t" = xyes; then : else { $as_echo "$as_me:${as_lineno-$LINENO}: checking for socklen_t equivalent" >&5 $as_echo_n "checking for socklen_t equivalent... " >&6; } if ${gl_cv_socklen_t_equiv+:} false; then : $as_echo_n "(cached) " >&6 else # Systems have either "struct sockaddr *" or # "void *" as the second argument to getpeername gl_cv_socklen_t_equiv= for arg2 in "struct sockaddr" void; do for t in int size_t "unsigned int" "long int" "unsigned long int"; do cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include int getpeername (int, $arg2 *, $t *); int main () { $t len; getpeername (0, 0, &len); ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_socklen_t_equiv="$t" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$gl_cv_socklen_t_equiv" != "" && break done test "$gl_cv_socklen_t_equiv" != "" && break done fi if test "$gl_cv_socklen_t_equiv" = ""; then as_fn_error $? "Cannot find a type to use in place of socklen_t" "$LINENO" 5 fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_socklen_t_equiv" >&5 $as_echo "$gl_cv_socklen_t_equiv" >&6; } cat >>confdefs.h <<_ACEOF #define socklen_t $gl_cv_socklen_t_equiv _ACEOF fi case "$host_os" in mingw*) REPLACE_STAT=1 ;; *) { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether stat handles trailing slashes on files" >&5 $as_echo_n "checking whether stat handles trailing slashes on files... " >&6; } if ${gl_cv_func_stat_file_slash+:} false; then : $as_echo_n "(cached) " >&6 else touch conftest.tmp # Assume that if we have lstat, we can also check symlinks. if test $ac_cv_func_lstat = yes; then ln -s conftest.tmp conftest.lnk fi if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_stat_file_slash="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_stat_file_slash="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { int result = 0; struct stat st; if (!stat ("conftest.tmp/", &st)) result |= 1; #if HAVE_LSTAT if (!stat ("conftest.lnk/", &st)) result |= 2; #endif return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_stat_file_slash=yes else gl_cv_func_stat_file_slash=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.tmp conftest.lnk fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_stat_file_slash" >&5 $as_echo "$gl_cv_func_stat_file_slash" >&6; } case $gl_cv_func_stat_file_slash in *no) REPLACE_STAT=1 $as_echo "#define REPLACE_FUNC_STAT_FILE 1" >>confdefs.h ;; esac case $host_os in solaris*) REPLACE_FSTAT=1 ;; esac ;; esac if test $REPLACE_STAT = 1; then gltests_LIBOBJS="$gltests_LIBOBJS stat.$ac_objext" case "$host_os" in mingw*) gltests_LIBOBJS="$gltests_LIBOBJS stat-w32.$ac_objext" ;; esac : fi if test "$GNULIB_STAT" != 1; then if test "$GNULIB_STAT" = 0; then GNULIB_STAT=$gl_module_indicator_condition else GNULIB_STAT="($GNULIB_STAT || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_STAT 1" >>confdefs.h ac_fn_c_check_member "$LINENO" "struct stat" "st_atim.tv_nsec" "ac_cv_member_struct_stat_st_atim_tv_nsec" "#include #include " if test "x$ac_cv_member_struct_stat_st_atim_tv_nsec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_ATIM_TV_NSEC 1 _ACEOF { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether struct stat.st_atim is of type struct timespec" >&5 $as_echo_n "checking whether struct stat.st_atim is of type struct timespec... " >&6; } if ${ac_cv_typeof_struct_stat_st_atim_is_struct_timespec+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_SYS_TIME_H # include #endif #include struct timespec ts; struct stat st; int main () { st.st_atim = ts; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : ac_cv_typeof_struct_stat_st_atim_is_struct_timespec=yes else ac_cv_typeof_struct_stat_st_atim_is_struct_timespec=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_typeof_struct_stat_st_atim_is_struct_timespec" >&5 $as_echo "$ac_cv_typeof_struct_stat_st_atim_is_struct_timespec" >&6; } if test $ac_cv_typeof_struct_stat_st_atim_is_struct_timespec = yes; then $as_echo "#define TYPEOF_STRUCT_STAT_ST_ATIM_IS_STRUCT_TIMESPEC 1" >>confdefs.h fi else ac_fn_c_check_member "$LINENO" "struct stat" "st_atimespec.tv_nsec" "ac_cv_member_struct_stat_st_atimespec_tv_nsec" "#include #include " if test "x$ac_cv_member_struct_stat_st_atimespec_tv_nsec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_ATIMESPEC_TV_NSEC 1 _ACEOF else ac_fn_c_check_member "$LINENO" "struct stat" "st_atimensec" "ac_cv_member_struct_stat_st_atimensec" "#include #include " if test "x$ac_cv_member_struct_stat_st_atimensec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_ATIMENSEC 1 _ACEOF else ac_fn_c_check_member "$LINENO" "struct stat" "st_atim.st__tim.tv_nsec" "ac_cv_member_struct_stat_st_atim_st__tim_tv_nsec" "#include #include " if test "x$ac_cv_member_struct_stat_st_atim_st__tim_tv_nsec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_ATIM_ST__TIM_TV_NSEC 1 _ACEOF fi fi fi fi ac_fn_c_check_member "$LINENO" "struct stat" "st_birthtimespec.tv_nsec" "ac_cv_member_struct_stat_st_birthtimespec_tv_nsec" "#include #include " if test "x$ac_cv_member_struct_stat_st_birthtimespec_tv_nsec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_BIRTHTIMESPEC_TV_NSEC 1 _ACEOF else ac_fn_c_check_member "$LINENO" "struct stat" "st_birthtimensec" "ac_cv_member_struct_stat_st_birthtimensec" "#include #include " if test "x$ac_cv_member_struct_stat_st_birthtimensec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_BIRTHTIMENSEC 1 _ACEOF else ac_fn_c_check_member "$LINENO" "struct stat" "st_birthtim.tv_nsec" "ac_cv_member_struct_stat_st_birthtim_tv_nsec" "#include #include " if test "x$ac_cv_member_struct_stat_st_birthtim_tv_nsec" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_STRUCT_STAT_ST_BIRTHTIM_TV_NSEC 1 _ACEOF fi fi fi if test $ac_cv_have_decl_strerror_r = no; then HAVE_DECL_STRERROR_R=0 fi if test $ac_cv_func_strerror_r = yes; then if test "$ERRNO_H:$REPLACE_STRERROR_0" = :0; then if test $gl_cv_func_strerror_r_posix_signature = yes; then case "$gl_cv_func_strerror_r_works" in *no) REPLACE_STRERROR_R=1 ;; esac else REPLACE_STRERROR_R=1 fi else REPLACE_STRERROR_R=1 fi fi if test $HAVE_DECL_STRERROR_R = 0 || test $REPLACE_STRERROR_R = 1; then gltests_LIBOBJS="$gltests_LIBOBJS strerror_r.$ac_objext" fi if test "$GNULIB_STRERROR_R" != 1; then if test "$GNULIB_STRERROR_R" = 0; then GNULIB_STRERROR_R=$gl_module_indicator_condition else GNULIB_STRERROR_R="($GNULIB_STRERROR_R || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_STRERROR_R 1" >>confdefs.h cat >>confdefs.h <<_ACEOF #define GNULIB_STRERROR_R_POSIX $gl_module_indicator_condition _ACEOF # Check for mmap(). Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. ac_fn_c_check_func "$LINENO" "mmap" "ac_cv_func_mmap" if test "x$ac_cv_func_mmap" = xyes; then : gl_have_mmap=yes else gl_have_mmap=no fi # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then { $as_echo "$as_me:${as_lineno-$LINENO}: checking for MAP_ANONYMOUS" >&5 $as_echo_n "checking for MAP_ANONYMOUS... " >&6; } cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef MAP_ANONYMOUS I cannot identify this map #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "I cannot identify this map" >/dev/null 2>&1; then : gl_have_mmap_anonymous=yes fi rm -f conftest* if test $gl_have_mmap_anonymous != yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #ifdef MAP_ANON I cannot identify this map #endif _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "I cannot identify this map" >/dev/null 2>&1; then : $as_echo "#define MAP_ANONYMOUS MAP_ANON" >>confdefs.h gl_have_mmap_anonymous=yes fi rm -f conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_have_mmap_anonymous" >&5 $as_echo "$gl_have_mmap_anonymous" >&6; } if test $gl_have_mmap_anonymous = yes; then $as_echo "#define HAVE_MAP_ANONYMOUS 1" >>confdefs.h fi fi if test $ac_cv_func_symlink = no; then HAVE_SYMLINK=0 else { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether symlink handles trailing slash correctly" >&5 $as_echo_n "checking whether symlink handles trailing slash correctly... " >&6; } if ${gl_cv_func_symlink_works+:} false; then : $as_echo_n "(cached) " >&6 else if test "$cross_compiling" = yes; then : case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_symlink_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_symlink_works="guessing no" ;; esac else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { int result = 0; if (!symlink ("a", "conftest.link/")) result |= 1; if (symlink ("conftest.f", "conftest.lnk2")) result |= 2; else if (!symlink ("a", "conftest.lnk2/")) result |= 4; return result; ; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_symlink_works=yes else gl_cv_func_symlink_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi rm -f conftest.f conftest.link conftest.lnk2 fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_symlink_works" >&5 $as_echo "$gl_cv_func_symlink_works" >&6; } case "$gl_cv_func_symlink_works" in *yes) ;; *) REPLACE_SYMLINK=1 ;; esac fi if test $HAVE_SYMLINK = 0 || test $REPLACE_SYMLINK = 1; then gltests_LIBOBJS="$gltests_LIBOBJS symlink.$ac_objext" fi if test "$GNULIB_SYMLINK" != 1; then if test "$GNULIB_SYMLINK" = 0; then GNULIB_SYMLINK=$gl_module_indicator_condition else GNULIB_SYMLINK="($GNULIB_SYMLINK || $gl_module_indicator_condition)" fi fi $as_echo "#define GNULIB_TEST_SYMLINK 1" >>confdefs.h if test $ac_cv_header_sys_ioctl_h = yes; then HAVE_SYS_IOCTL_H=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether declares ioctl" >&5 $as_echo_n "checking whether declares ioctl... " >&6; } if ${gl_cv_decl_ioctl_in_sys_ioctl_h+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { (void) ioctl; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gl_cv_decl_ioctl_in_sys_ioctl_h=yes else gl_cv_decl_ioctl_in_sys_ioctl_h=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_decl_ioctl_in_sys_ioctl_h" >&5 $as_echo "$gl_cv_decl_ioctl_in_sys_ioctl_h" >&6; } else HAVE_SYS_IOCTL_H=0 fi if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_ioctl_h='<'sys/ioctl.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_ioctl_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_ioctl_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/ioctl.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_ioctl_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_ioctl_h gl_cv_next_sys_ioctl_h='"'$gl_header'"' else gl_cv_next_sys_ioctl_h='<'sys/ioctl.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_ioctl_h" >&5 $as_echo "$gl_cv_next_sys_ioctl_h" >&6; } fi NEXT_SYS_IOCTL_H=$gl_cv_next_sys_ioctl_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/ioctl.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_ioctl_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H=$gl_next_as_first_directive for gl_func in ioctl; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include /* Some platforms declare ioctl in the wrong header. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include #endif int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_stat_h='<'sys/stat.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_stat_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_stat_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/stat.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_stat_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_stat_h gl_cv_next_sys_stat_h='"'$gl_header'"' else gl_cv_next_sys_stat_h='<'sys/stat.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_stat_h" >&5 $as_echo "$gl_cv_next_sys_stat_h" >&6; } fi NEXT_SYS_STAT_H=$gl_cv_next_sys_stat_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/stat.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_stat_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H=$gl_next_as_first_directive WINDOWS_STAT_TIMESPEC=0 ac_fn_c_check_type "$LINENO" "nlink_t" "ac_cv_type_nlink_t" "#include #include " if test "x$ac_cv_type_nlink_t" = xyes; then : else $as_echo "#define nlink_t int" >>confdefs.h fi for gl_func in fchmodat fstat fstatat futimens lchmod lstat mkdirat mkfifo mkfifoat mknod mknodat stat utimensat; do as_gl_Symbol=`$as_echo "gl_cv_have_raw_decl_$gl_func" | $as_tr_sh` { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether $gl_func is declared without a macro" >&5 $as_echo_n "checking whether $gl_func is declared without a macro... " >&6; } if eval \${$as_gl_Symbol+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include int main () { #undef $gl_func (void) $gl_func; ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : eval "$as_gl_Symbol=yes" else eval "$as_gl_Symbol=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi eval ac_res=\$$as_gl_Symbol { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_res" >&5 $as_echo "$ac_res" >&6; } if eval test \"x\$"$as_gl_Symbol"\" = x"yes"; then : cat >>confdefs.h <<_ACEOF #define `$as_echo "HAVE_RAW_DECL_$gl_func" | $as_tr_cpp` 1 _ACEOF eval ac_cv_have_decl_$gl_func=yes fi done if test $gl_cv_have_include_next = yes; then gl_cv_next_sys_uio_h='<'sys/uio.h'>' else { $as_echo "$as_me:${as_lineno-$LINENO}: checking absolute name of " >&5 $as_echo_n "checking absolute name of ... " >&6; } if ${gl_cv_next_sys_uio_h+:} false; then : $as_echo_n "(cached) " >&6 else if test $ac_cv_header_sys_uio_h = yes; then cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include _ACEOF case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac case "$host_os" in mingw*) gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo 'sys/uio.h' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' gl_cv_absolute_sys_uio_h=`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&5 | sed -n "$gl_absolute_header_sed"` gl_header=$gl_cv_absolute_sys_uio_h gl_cv_next_sys_uio_h='"'$gl_header'"' else gl_cv_next_sys_uio_h='<'sys/uio.h'>' fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_next_sys_uio_h" >&5 $as_echo "$gl_cv_next_sys_uio_h" >&6; } fi NEXT_SYS_UIO_H=$gl_cv_next_sys_uio_h if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'sys/uio.h'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=$gl_cv_next_sys_uio_h fi NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H=$gl_next_as_first_directive if test $ac_cv_header_sys_uio_h = yes; then HAVE_SYS_UIO_H=1 else HAVE_SYS_UIO_H=0 fi if test $gl_threads_api = posix; then gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" for ac_func in pthread_atfork do : ac_fn_c_check_func "$LINENO" "pthread_atfork" "ac_cv_func_pthread_atfork" if test "x$ac_cv_func_pthread_atfork" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_PTHREAD_ATFORK 1 _ACEOF fi done LIBS="$gl_save_LIBS" fi if test $ac_cv_have_decl_unsetenv = no; then HAVE_DECL_UNSETENV=0 fi for ac_func in unsetenv do : ac_fn_c_check_func "$LINENO" "unsetenv" "ac_cv_func_unsetenv" if test "x$ac_cv_func_unsetenv" = xyes; then : cat >>confdefs.h <<_ACEOF #define HAVE_UNSETENV 1 _ACEOF fi done if test $ac_cv_func_unsetenv = no; then HAVE_UNSETENV=0 else HAVE_UNSETENV=1 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for unsetenv() return type" >&5 $as_echo_n "checking for unsetenv() return type... " >&6; } if ${gt_cv_func_unsetenv_ret+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #undef _BSD #define _BSD 1 /* unhide unsetenv declaration in OSF/1 5.1 */ #include extern #ifdef __cplusplus "C" #endif int unsetenv (const char *name); int main () { ; return 0; } _ACEOF if ac_fn_c_try_compile "$LINENO"; then : gt_cv_func_unsetenv_ret='int' else gt_cv_func_unsetenv_ret='void' fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_func_unsetenv_ret" >&5 $as_echo "$gt_cv_func_unsetenv_ret" >&6; } if test $gt_cv_func_unsetenv_ret = 'void'; then $as_echo "#define VOID_UNSETENV 1" >>confdefs.h REPLACE_UNSETENV=1 fi { $as_echo "$as_me:${as_lineno-$LINENO}: checking whether unsetenv obeys POSIX" >&5 $as_echo_n "checking whether unsetenv obeys POSIX... 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Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; # if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; # endif return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr" >&5 $as_echo "$gt_cv_locale_fr" >&6; } LOCALE_FR=$gt_cv_locale_fr { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a french Unicode locale" >&5 $as_echo_n "checking for a french Unicode locale... " >&6; } if ${gt_cv_locale_fr_utf8+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_fr_utf8" >&5 $as_echo "$gt_cv_locale_fr_utf8" >&6; } LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a traditional japanese locale" >&5 $as_echo_n "checking for a traditional japanese locale... " >&6; } if ${gt_cv_locale_ja+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gt_cv_locale_ja" >&5 $as_echo "$gt_cv_locale_ja" >&6; } LOCALE_JA=$gt_cv_locale_ja { $as_echo "$as_me:${as_lineno-$LINENO}: checking for a transitional chinese locale" >&5 $as_echo_n "checking for a transitional chinese locale... " >&6; } if ${gt_cv_locale_zh_CN+:} false; then : $as_echo_n "(cached) " >&6 else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; #endif } _ACEOF if { { eval echo "\"\$as_me\":${as_lineno-$LINENO}: \"$ac_link\""; } >&5 (eval $ac_link) 2>&5 ac_status=$? $as_echo "$as_me:${as_lineno-$LINENO}: \$? = $ac_status" >&5 test $ac_status = 0; } && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. 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BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include register long global __asm__ ("%ebx"); int main () { setlocale (LC_ALL, "en_US.UTF-8"); global = 0x12345678; if (wctob (0x00FC) != -1) return 1; if (global != 0x12345678) return 2; return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : : else gl_cv_func_wctob_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi ;; esac if test "$gl_cv_func_wctob_works" != no && test $LOCALE_FR != none; then if test "$cross_compiling" = yes; then : : else cat confdefs.h - <<_ACEOF >conftest.$ac_ext /* end confdefs.h. */ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { wchar_t wc; if (mbtowc (&wc, "\374", 1) == 1) if (wctob (wc) != (unsigned char) '\374') return 1; } return 0; } _ACEOF if ac_fn_c_try_run "$LINENO"; then : gl_cv_func_wctob_works=yes else gl_cv_func_wctob_works=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext \ conftest.$ac_objext conftest.beam conftest.$ac_ext fi fi fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $gl_cv_func_wctob_works" >&5 $as_echo "$gl_cv_func_wctob_works" >&6; } case "$gl_cv_func_wctob_works" in *yes) ;; *) REPLACE_WCTOB=1 ;; esac if test $REPLACE_WCTOB = 0; then ac_fn_c_check_decl "$LINENO" "wctob" "ac_cv_have_decl_wctob" " /* Tru64 with Desktop Toolkit C has a bug: must be included before . 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As described in the output # `bootstrapped/m4/gnulib-common.m4', this is only necessary until Autoconf # 2.70 is released. Afterwards, we can use AC_C_RESTRICT. if test "x$ac_cv_c_restrict" = "xno"; then : gal_restrict_replace= else gal_restrict_replace=$ac_cv_c_restrict fi RESTRICT_REPLACEMENT=$gal_restrict_replace # To add the help2man: # Extract the first word of "help2man", so it can be a program name with args. set dummy help2man; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... 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Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char git_libgit2_init (); int main () { return git_libgit2_init (); ; return 0; } _ACEOF for ac_lib in '' git2; do if test -z "$ac_lib"; then ac_res="none required" else ac_res=-l$ac_lib LIBS="-l$ac_lib $ac_func_search_save_LIBS" fi if ac_fn_c_try_link "$LINENO"; then : ac_cv_search_git_libgit2_init=$ac_res fi rm -f core conftest.err conftest.$ac_objext \ conftest$ac_exeext if ${ac_cv_search_git_libgit2_init+:} false; then : break fi done if ${ac_cv_search_git_libgit2_init+:} false; then : else ac_cv_search_git_libgit2_init=no fi rm conftest.$ac_ext LIBS=$ac_func_search_save_LIBS fi { $as_echo "$as_me:${as_lineno-$LINENO}: result: $ac_cv_search_git_libgit2_init" >&5 $as_echo "$ac_cv_search_git_libgit2_init" >&6; } ac_res=$ac_cv_search_git_libgit2_init if test "$ac_res" != no; then : test "$ac_res" = "none required" || LIBS="$ac_res $LIBS" has_libgit2=1 else has_libgit2=0 fi cat >>confdefs.h <<_ACEOF #define GAL_CONFIG_HAVE_LIBGIT2 $has_libgit2 _ACEOF if test "x$has_libgit2" = "x1"; then : else anywarnings=yes fi HAVE_LIBGIT2=$has_libgit2 # Check the libtool executable on the system. Note that Gnuastro also ships # with a version of Libtool. We don't want Gnuastro's Libtool, here we want # to see if the system has libtool independent of Gnuastro so BuildProgram # can use it later. # Extract the first word of "libtool", so it can be a program name with args. set dummy libtool; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... 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Make sure we have at least that version. # # Below, only when Ghostscript exists, we check its version and only if its # version is larger than 9.10, does Gnuastro finally assume the existence # of Ghostscript. AX_COMPARE_VERSION comes from the GNU Autoconf Archive's # ax_compare_version.m4. # Extract the first word of "gs", so it can be a program name with args. set dummy gs; ac_word=$2 { $as_echo "$as_me:${as_lineno-$LINENO}: checking for $ac_word" >&5 $as_echo_n "checking for $ac_word... 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$SED "$delay_single_quote_subst"`' export_symbols_cmds_CXX='`$ECHO "$export_symbols_cmds_CXX" | $SED "$delay_single_quote_subst"`' exclude_expsyms_CXX='`$ECHO "$exclude_expsyms_CXX" | $SED "$delay_single_quote_subst"`' include_expsyms_CXX='`$ECHO "$include_expsyms_CXX" | $SED "$delay_single_quote_subst"`' prelink_cmds_CXX='`$ECHO "$prelink_cmds_CXX" | $SED "$delay_single_quote_subst"`' postlink_cmds_CXX='`$ECHO "$postlink_cmds_CXX" | $SED "$delay_single_quote_subst"`' file_list_spec_CXX='`$ECHO "$file_list_spec_CXX" | $SED "$delay_single_quote_subst"`' hardcode_action_CXX='`$ECHO "$hardcode_action_CXX" | $SED "$delay_single_quote_subst"`' compiler_lib_search_dirs_CXX='`$ECHO "$compiler_lib_search_dirs_CXX" | $SED "$delay_single_quote_subst"`' predep_objects_CXX='`$ECHO "$predep_objects_CXX" | $SED "$delay_single_quote_subst"`' postdep_objects_CXX='`$ECHO "$postdep_objects_CXX" | $SED "$delay_single_quote_subst"`' predeps_CXX='`$ECHO "$predeps_CXX" | $SED "$delay_single_quote_subst"`' 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The executable names searched were \`libtool'" $as_echo " and \`glibtool'." $as_echo if test "x$has_libtool" = "xyes"; then : $as_echo " -- A libtool implementation was found, but it isn't GNU." $as_echo fi fi if test "x$has_ghostscript" = "xno"; then : $as_echo " - GPL GhostScript version 9.10 or later, with the executable" $as_echo " name \`gs', was not found in your PATH environment variable." $as_echo " If PDF outputs are desired from ConvertType, it will abort" $as_echo " with an EPS output which you can convert to PDF by other means." $as_echo fi # The last two scenarios described below are taken from # https://unix.stackexchange.com/questions/65700/is-it-safe-to-add-to-my-path-how-come if test "x$path_warning" = "xyes"; then : $as_echo " - Your PATH contains the current directory. This does not affect" $as_echo " this build and installation of Gnuastro in any way, it is just to" $as_echo " to remind you that this is a security risk." $as_echo " It is a very serious security risk if it is closer to the start" $as_echo " of your PATH: a malicious/wrong program might be run instead of" $as_echo " a desired program, someone might find out you frequently mistype" $as_echo " a command and install a matching one, someone might install a" $as_echo " fake command with the name of one that is not installed. You can" $as_echo " always run a program in the current directory by explicity adding" $as_echo " a \`./' before it's name. Run the following command after" $as_echo " installing Gnuastro to learn more about PATH:" $as_echo " $ info gnuastro \"Installation directory\"" $as_echo fi $as_echo " All checks related to the warning(s) above will be skipped." $as_echo fi $as_echo "To build Gnuastro $PACKAGE_VERSION, please run:" $as_echo $as_echo " make -j8" $as_echo $as_echo "(You can change the 8 to the number of CPU threads available.)" $as_echo "(Configure with '--disable-guide-message' for no messages.)" $as_echo "(Please be patient, some libraries can take a few minutes to compile.)" $as_echo ======================================================================= $as_echo ======================================================================= $as_echo fi gnuastro-0.5/Makefile.am0000644000175000017500000003441013211076737012206 00000000000000## Process this file with automake to produce Makefile.in ## ## Hand written file: used as input into Autotools. ## This is part of GNU Astronomy Utilities (gnuastro). ## ## Original author: ## Mohammad Akhlaghi ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see . ## Sources to be created before everything else ## ============================================ ## ## These target(s) will be created before anything else when running ## `make', `make check', or `make install', see the "Built sources" section ## of the AUTOMAKE manual and the git-version-gen script comments for more ## information. Note that AUTHORS depends on `$(top_srcdir)/.version', and ## `$(top_srcdir)/.version' depends on $(top_srcdir)/configure'. So any ## time the version is updated, both of these will be re-built. But during ## usual utility and library development, `$(top_srcdir)/configure' is not ## commonly updated, so this will not slow down the process. BUILT_SOURCES = $(top_srcdir)/AUTHORS ## Directories to check: ## ===================== ## ## Gnulib is intentionally compiled and tested prior to the gnuastro ## progams. With this configuration, the user can confirm if the ## problem is internal to gnulib or still persists after all the ## Gnulib tests have been done. if COND_ARITHMETIC MAYBE_ARITHMETIC = bin/arithmetic endif if COND_BUILDPROG MAYBE_BUILDPROG = bin/buildprog endif if COND_CONVERTT MAYBE_CONVERTT = bin/convertt endif if COND_CONVOLVE MAYBE_CONVOLVE = bin/convolve endif if COND_COSMICCAL MAYBE_COSMICCAL = bin/cosmiccal endif if COND_CROP MAYBE_CROP = bin/crop endif if COND_FITS MAYBE_FITS = bin/fits endif if COND_MATCH MAYBE_MATCH = bin/match endif if COND_MKCATALOG MAYBE_MKCATALOG = bin/mkcatalog endif if COND_MKNOISE MAYBE_MKNOISE = bin/mknoise endif if COND_MKPROF MAYBE_MKPROF = bin/mkprof endif if COND_NOISECHISEL MAYBE_NOISECHISEL = bin/noisechisel endif if COND_STATISTICS MAYBE_STATISTICS = bin/statistics endif if COND_TABLE MAYBE_TABLE = bin/table endif #if COND_TEMPLATE # MAYBE_TEMPLATE = bin/TEMPLATE #endif if COND_WARP MAYBE_WARP = bin/warp endif if COND_GNULIBCHECK MAYBE_GNULIBCHECK = bootstrapped/tests endif ## Subdirectories to build ## ======================= ## ## Note that by default `COND_TEMPLATE' is not set in configure, it is ## commented, and exists only as a template for you to copy and paste to ## name your new utility. The same rule is applied here (in the `if' ## conditions above). When `MAYBE_TEMPLATE' is not defined, then Make will ## see it as a blank string and igonore it, so there is no problem with ## having an uncommented `MAYBE_TEMPLATE' as a value in `SUBDIRS'. SUBDIRS = bootstrapped/lib $(MAYBE_GNULIBCHECK) lib $(MAYBE_ARITHMETIC) \ $(MAYBE_BUILDPROG) $(MAYBE_CONVERTT) $(MAYBE_CONVOLVE) \ $(MAYBE_COSMICCAL) $(MAYBE_CROP) $(MAYBE_FITS) $(MAYBE_MATCH) \ $(MAYBE_MKCATALOG) $(MAYBE_MKNOISE) $(MAYBE_MKPROF) \ $(MAYBE_NOISECHISEL) $(MAYBE_STATISTICS) $(MAYBE_TABLE) \ $(MAYBE_TEMPLATE) $(MAYBE_WARP) doc tests ## Add m4/ to the list of directories to search for m4 files ## ========================================================= ACLOCAL_AMFLAGS = -I bootstrapped/m4 ## Files that are installed (and distributed) ## ========================================= dist_doc_DATA = README # Installed system configuration files # ==================================== dist_sysconf_DATA = bin/gnuastro.conf ## Files that are only distributed ## =============================== EXTRA_DIST = genauthors .dir-locals.el .version tmpfs-config-make \ bootstrapped/README .autom4te.cfg ## Print the completion messages ## ============================= ## ## After the jobs in all the subdirectories are done, print the following ## messages to confirm that everything is complete and guide the users on ## what they should do next. ## ## When running ./configure, the user can opt-out of these messages using ## the GUIDEMESSAGE variable that is set when they run ./configure with the ## `--distable-guide-message' option. ## ## Note that all-local is a prerequisite of `make check' too, so we will ## only print its message when `make' was called with no options. Make will ## set MAKECMDGOALS to blank if there are no arguments, however, the way ## Automake works, its value is set to "all-am". all-local: @if [ x$(MAKECMDGOALS) = x"all-am" ] && [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo "Gnuastro $(VERSION), was successfully built."; \ echo "Please check the build on your system by running:"; \ echo; \ echo " make check -j8"; \ echo; \ echo "(You can change the 8 to the number of CPU threads available.)"; \ echo "(The following \"Leaving directory\" notices can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi ## We cannot do the writing persmission test at configure time. Here is a ## quote from the generated ./configure script: The prefix variables... ## ## "... are left unexpanded so users can "make install exec_prefix=/foo" ## and all the variables that are supposed to be based on exec_prefix by ## default will actually change." ## ## So actually, they can also do that after `make check'. Usually ## professional users would want to do such a thing, so they can ignore the ## NOTE. This note is mostly for beginners and it is not written to convey ## that this is the ONLY solution. check-local: @if [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo "Your build of Gnuastro $(VERSION) didn't fail on any tests."; \ echo "To install Gnuastro, please run the command(s) below:"; \ echo; \ if [ ! -w $(prefix) ] ; then \ echo "(NOTE: As the user $$USER, you don't have writing permissions"; \ echo "in \"$(prefix)\". To install Gnuastro there, you must get "; \ echo "privileges first, as described below. If you can't, configure "; \ echo "Gnuastro again, for example: \"./configure --prefix ~/.local\".)"; \ echo; \ echo " sudo make install"; \ echo "or"; \ echo " su"; \ fi; \ echo " make install"; \ if [ ! -w $(prefix) ] ; then \ echo " exit"; \ fi; \ echo; \ echo "(The following \"Leaving directory\" notices can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi ## Note that the `\' characters in the GNU head here are not printed on the ## command line. So we have to consider them. The ASCII GNU head is taken ## from: https://www.gnu.org/graphics/gnu-ascii.html install-exec-local: @if [ x$(GUIDEMESSAGE) = xyes ]; then \ echo; \ echo "==================================================================="; \ echo "==================================================================="; \ echo " , , "; \ echo " / \ "; \ echo " ((__-^^-,-^^-__)) Congratulations!"; \ echo " \`-_---' \`---_-' GNU Astronomy Utilities (Gnuastro),"; \ echo " \`--|o\` 'o|--' Version $(VERSION)"; \ echo " \ \` / "; \ echo " ): :( Successfully installed on this system."; \ echo " :o_o: "; \ echo " \"-\" "; \ echo; \ echo "More information Command to run "; \ echo "---------------- -------------- "; \ echo "Complete official Gnuastro book: ' info gnuastro '"; \ echo "Entertaining tutorials: ' info gnuastro Tutorials '"; \ echo "Dedicated help mailing list: ' info help-gnuastro '"; \ echo "Instructions for reporting bugs: ' info bug-gnuastro '"; \ echo "Effectively use Info: ' info info '"; \ echo; \ echo; \ echo "Environment variables to check: "; \ echo " - '$(prefix)/bin' in PATH."; \ echo " - '$(prefix)/lib' in LD_LIBRARY_PATH."; \ echo "(for an intro, run 'info gnuastro \"Installation directory\"')"; \ echo; \ echo; \ echo "To stay up to date with future releases, please subscribe to: "; \ echo " https://lists.gnu.org/mailman/listinfo/info-gnuastro"; \ echo; \ echo; \ echo "(The following lines can be ignored.)"; \ echo "==================================================================="; \ echo "==================================================================="; \ echo; \ fi ## $(top_srcdir)/.version ## ====================== ## ## This file is created from the $(VERSION) variable which was defined by ## the `git-version-gen' script (located at address below), which is run ## when the `$(top_srcdir)/configure' script is being built by Autoconf. ## ## $(top_srcdir)/bootstrapped/build-aux/git-version-gen ## ## Note that contrary to what is proposed by `git-version-gen', here the ## creation of `$(top_srcdir)/.version' depends on the ## `$(top_srcdir)/configure' script. Therefore, anytime a the VERSION ## variable is updated there, `$(top_srcdir)/.version' is also ## updated. During development, of the main functionality of Gnuastro ## (utilities and libraries), the `$(top_srcdir/configure' script is rarely ## updated, so `$(top_srcdir)/.version' will not be rebuilt and thus it ## won't harm the speed of tests during development. $(top_srcdir)/.version: $(top_srcdir)/configure echo $(VERSION) > $@-t && mv $@-t $@ ## $(top_srcdir)/AUTHORS ## ===================== ## ## This file is generated automatically from the version controlled ## history. Note the following: ## ## - `$(top_srcdir)/AUTHORS' is defined as a BUILT_SOURCES variable, so ## it is the first thing that is built (even in multi-threaded runs). ## ## - `$(top_srcdir)/AUTHORS' is updated only when ## `$(top_srcdir)/.version' is updated. `$(top_srcdir)/.version' its ## self is only updated when `$(top_srcdir)/configure' is updated. But ## generally, the `$(top_srcdir)/configure' script is not updated ## regularly during development and outside of version control. ## ## - The `$(top_srcdir)/genauthors' script will not do anything ## (make/update the `$(top_srcdir)AUTHORS' file) when there is no git ## repository. `$(top_srcdir)/AUTHORS' is only necessary when building ## a tarball distribution. $(top_srcdir)/AUTHORS: $(top_srcdir)/.version $(top_srcdir)/genauthors $(top_srcdir) ## Run when building a distribution ## ================================ ## ## These targets will be created when building a (tarball) ## distribution. Note that AUTHORS depends on `.version'. dist-hook: $(top_srcdir)/AUTHORS echo $(VERSION) > $(distdir)/.tarball-version ## Nice joke ## ========= ## ## This joke is taken from the "The art of unix programming", and a quote ## by Stuart Feldman (creator of Make): "One of the older Unix jokes is ## "Make love" which results in "Don’t know how to make love"." love: @echo "Don't know how to make love!" gnuastro-0.5/bootstrapped/0000755000175000017500000000000013217220467012733 500000000000000gnuastro-0.5/bootstrapped/doc/0000755000175000017500000000000013217220467013500 500000000000000gnuastro-0.5/bootstrapped/doc/fdl.texi0000644000175000017500000005561213217200020015050 00000000000000@c The GNU Free Documentation License. @center Version 1.3, 3 November 2008 @c This file is intended to be included within another document, @c hence no sectioning command or @node. @display Copyright @copyright{} 2000, 2001, 2002, 2007, 2008 Free Software Foundation, Inc. @uref{https://fsf.org/} Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. @end display @enumerate 0 @item PREAMBLE The purpose of this License is to make a manual, textbook, or other functional and useful document @dfn{free} in the sense of freedom: to assure everyone the effective freedom to copy and redistribute it, with or without modifying it, either commercially or noncommercially. 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A ``Massive Multiauthor Collaboration'' (or ``MMC'') contained in the site means any set of copyrightable works thus published on the MMC site. ``CC-BY-SA'' means the Creative Commons Attribution-Share Alike 3.0 license published by Creative Commons Corporation, a not-for-profit corporation with a principal place of business in San Francisco, California, as well as future copyleft versions of that license published by that same organization. ``Incorporate'' means to publish or republish a Document, in whole or in part, as part of another Document. An MMC is ``eligible for relicensing'' if it is licensed under this License, and if all works that were first published under this License somewhere other than this MMC, and subsequently incorporated in whole or in part into the MMC, (1) had no cover texts or invariant sections, and (2) were thus incorporated prior to November 1, 2008. The operator of an MMC Site may republish an MMC contained in the site under CC-BY-SA on the same site at any time before August 1, 2009, provided the MMC is eligible for relicensing. @end enumerate @page @heading ADDENDUM: How to use this License for your documents To use this License in a document you have written, include a copy of the License in the document and put the following copyright and license notices just after the title page: @smallexample @group Copyright (C) @var{year} @var{your name}. Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled ``GNU Free Documentation License''. @end group @end smallexample If you have Invariant Sections, Front-Cover Texts and Back-Cover Texts, replace the ``with@dots{}Texts.''@: line with this: @smallexample @group with the Invariant Sections being @var{list their titles}, with the Front-Cover Texts being @var{list}, and with the Back-Cover Texts being @var{list}. @end group @end smallexample If you have Invariant Sections without Cover Texts, or some other combination of the three, merge those two alternatives to suit the situation. If your document contains nontrivial examples of program code, we recommend releasing these examples in parallel under your choice of free software license, such as the GNU General Public License, to permit their use in free software. @c Local Variables: @c ispell-local-pdict: "ispell-dict" @c End: gnuastro-0.5/bootstrapped/tests/0000755000175000017500000000000013217220466014074 500000000000000gnuastro-0.5/bootstrapped/tests/xalloc-oversized.h0000644000175000017500000000442513217200024017450 00000000000000/* xalloc-oversized.h -- memory allocation size checking Copyright (C) 1990-2000, 2003-2004, 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef XALLOC_OVERSIZED_H_ #define XALLOC_OVERSIZED_H_ #include #include /* True if N * S would overflow in a size_t calculation, or would generate a value larger than PTRDIFF_MAX. This expands to a constant expression if N and S are both constants. By gnulib convention, SIZE_MAX represents overflow in size calculations, so the conservative size_t-based dividend to use here is SIZE_MAX - 1. */ #define __xalloc_oversized(n, s) \ ((size_t) (PTRDIFF_MAX < SIZE_MAX ? PTRDIFF_MAX : SIZE_MAX - 1) / (s) < (n)) #if PTRDIFF_MAX < SIZE_MAX typedef ptrdiff_t __xalloc_count_type; #else typedef size_t __xalloc_count_type; #endif /* Return 1 if an array of N objects, each of size S, cannot exist reliably due to size or ptrdiff_t arithmetic overflow. S must be positive and N must be nonnegative. This is a macro, not a function, so that it works correctly even when SIZE_MAX < N. */ #if 7 <= __GNUC__ # define xalloc_oversized(n, s) \ __builtin_mul_overflow_p (n, s, (__xalloc_count_type) 1) #elif 5 <= __GNUC__ && !defined __ICC && !__STRICT_ANSI__ # define xalloc_oversized(n, s) \ (__builtin_constant_p (n) && __builtin_constant_p (s) \ ? __xalloc_oversized (n, s) \ : ({ __xalloc_count_type __xalloc_count; \ __builtin_mul_overflow (n, s, &__xalloc_count); })) /* Other compilers use integer division; this may be slower but is more portable. */ #else # define xalloc_oversized(n, s) __xalloc_oversized (n, s) #endif #endif /* !XALLOC_OVERSIZED_H_ */ gnuastro-0.5/bootstrapped/tests/wctomb-impl.h0000644000175000017500000000211313217200024016400 00000000000000/* Convert wide character to multibyte character. Copyright (C) 2011-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ int wctomb (char *s, wchar_t wc) { if (s == NULL) return 0; else { mbstate_t state; size_t result; memset (&state, 0, sizeof (mbstate_t)); result = wcrtomb (s, wc, &state); if (result == (size_t)-1) return -1; return result; } } gnuastro-0.5/bootstrapped/tests/test-wcrtomb-w32-5.sh0000755000175000017500000000012013217200024017535 00000000000000#!/bin/sh # Test a CP936 locale. ./test-wcrtomb-w32${EXEEXT} Chinese_China 936 gnuastro-0.5/bootstrapped/tests/test-wcrtomb-w32-4.sh0000755000175000017500000000012113217200024017535 00000000000000#!/bin/sh # Test a CP950 locale. ./test-wcrtomb-w32${EXEEXT} Chinese_Taiwan 950 gnuastro-0.5/bootstrapped/tests/test-wcrtomb-w32-3.sh0000755000175000017500000000012113217200024017534 00000000000000#!/bin/sh # Test a CP932 locale. ./test-wcrtomb-w32${EXEEXT} Japanese_Japan 932 gnuastro-0.5/bootstrapped/tests/test-wcrtomb-w32-2.sh0000755000175000017500000000013213217200024017535 00000000000000#!/bin/sh # Test a CP1256 locale. ./test-wcrtomb-w32${EXEEXT} "Arabic_Saudi Arabia" 1256 gnuastro-0.5/bootstrapped/tests/test-wcrtomb-w32-1.sh0000755000175000017500000000012213217200024017533 00000000000000#!/bin/sh # Test a CP1252 locale. ./test-wcrtomb-w32${EXEEXT} French_France 1252 gnuastro-0.5/bootstrapped/tests/test-wcrtomb.sh0000755000175000017500000000136113217200024016772 00000000000000#!/bin/sh # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR \ ./test-wcrtomb${EXEEXT} 1 \ || exit 1 fi # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 != none; then LC_ALL=$LOCALE_FR_UTF8 \ ./test-wcrtomb${EXEEXT} 2 \ || exit 1 fi # Test whether a specific EUC-JP locale is installed. : ${LOCALE_JA=ja_JP} if test $LOCALE_JA != none; then LC_ALL=$LOCALE_JA \ ./test-wcrtomb${EXEEXT} 3 \ || exit 1 fi # Test whether a specific GB18030 locale is installed. : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_ZH_CN != none; then LC_ALL=$LOCALE_ZH_CN \ ./test-wcrtomb${EXEEXT} 4 \ || exit 1 fi exit 0 gnuastro-0.5/bootstrapped/tests/test-verify.sh0000755000175000017500000000132513217200024016621 00000000000000#!/bin/sh . "${srcdir=.}/init.sh" # We are not interested in triggering bugs in the compilers and tools # (such as gcc 4.3.1 on openSUSE 11.0). unset MALLOC_PERTURB_ # Rather than figure out how to invoke the compiler with the right # include path ourselves, we let make do it: (cd "$initial_cwd_" \ && rm -f test-verify-try.o \ && $MAKE test-verify-try.o >/dev/null 2>&1) \ || skip_ "cannot compile error-free" # Now, prove that we encounter all expected compilation failures: : >out : >err for i in 1 2 3 4 5; do (cd "$initial_cwd_" rm -f test-verify-try.o $MAKE CFLAGS=-DEXP_FAIL=$i test-verify-try.o) >>out 2>>err \ && { warn_ "compiler didn't detect verification failure $i"; fail=1; } done Exit $fail gnuastro-0.5/bootstrapped/tests/time.in.h0000644000175000017500000003134013217200024015515 00000000000000/* A more-standard . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Don't get in the way of glibc when it includes time.h merely to declare a few standard symbols, rather than to declare all the symbols. (However, skip this for MinGW as it treats __need_time_t incompatibly.) Also, Solaris 8 eventually includes itself recursively; if that is happening, just include the system without adding our own declarations. */ #if (((defined __need_time_t || defined __need_clock_t \ || defined __need_timespec) \ && !defined __MINGW32__) \ || defined _@GUARD_PREFIX@_TIME_H) # @INCLUDE_NEXT@ @NEXT_TIME_H@ #else # define _@GUARD_PREFIX@_TIME_H # @INCLUDE_NEXT@ @NEXT_TIME_H@ /* NetBSD 5.0 mis-defines NULL. */ # include /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Some systems don't define struct timespec (e.g., AIX 4.1, Ultrix 4.3). Or they define it with the wrong member names or define it in (e.g., FreeBSD circa 1997). Stock Mingw prior to 3.0 does not define it, but the pthreads-win32 library defines it in . */ # if ! @TIME_H_DEFINES_STRUCT_TIMESPEC@ # if @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ # include # elif @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ # include # elif @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ # include # else # ifdef __cplusplus extern "C" { # endif # if !GNULIB_defined_struct_timespec # undef timespec # define timespec rpl_timespec struct timespec { time_t tv_sec; long int tv_nsec; }; # define GNULIB_defined_struct_timespec 1 # endif # ifdef __cplusplus } # endif # endif # endif # if !GNULIB_defined_struct_time_t_must_be_integral /* Per http://austingroupbugs.net/view.php?id=327, POSIX requires time_t to be an integer type, even though C99 permits floating point. We don't know of any implementation that uses floating point, and it is much easier to write code that doesn't have to worry about that corner case, so we force the issue. */ struct __time_t_must_be_integral { unsigned int __floating_time_t_unsupported : (time_t) 1; }; # define GNULIB_defined_struct_time_t_must_be_integral 1 # endif /* Sleep for at least RQTP seconds unless interrupted, If interrupted, return -1 and store the remaining time into RMTP. See . */ # if @GNULIB_NANOSLEEP@ # if @REPLACE_NANOSLEEP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define nanosleep rpl_nanosleep # endif _GL_FUNCDECL_RPL (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp)); # else # if ! @HAVE_NANOSLEEP@ _GL_FUNCDECL_SYS (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (nanosleep, int, (struct timespec const *__rqtp, struct timespec *__rmtp)); # endif _GL_CXXALIASWARN (nanosleep); # endif /* Initialize time conversion information. */ # if @GNULIB_TZSET@ # if @REPLACE_TZSET@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef tzset # define tzset rpl_tzset # endif _GL_FUNCDECL_RPL (tzset, void, (void)); _GL_CXXALIAS_RPL (tzset, void, (void)); # else # if ! @HAVE_TZSET@ _GL_FUNCDECL_SYS (tzset, void, (void)); # endif _GL_CXXALIAS_SYS (tzset, void, (void)); # endif _GL_CXXALIASWARN (tzset); # endif /* Return the 'time_t' representation of TP and normalize TP. */ # if @GNULIB_MKTIME@ # if @REPLACE_MKTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mktime rpl_mktime # endif _GL_FUNCDECL_RPL (mktime, time_t, (struct tm *__tp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mktime, time_t, (struct tm *__tp)); # else _GL_CXXALIAS_SYS (mktime, time_t, (struct tm *__tp)); # endif _GL_CXXALIASWARN (mktime); # endif /* Convert TIMER to RESULT, assuming local time and UTC respectively. See and . */ # if @GNULIB_TIME_R@ # if @REPLACE_LOCALTIME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef localtime_r # define localtime_r rpl_localtime_r # endif _GL_FUNCDECL_RPL (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # else # if ! @HAVE_DECL_LOCALTIME_R@ _GL_FUNCDECL_SYS (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (localtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # endif # if @HAVE_DECL_LOCALTIME_R@ _GL_CXXALIASWARN (localtime_r); # endif # if @REPLACE_LOCALTIME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gmtime_r # define gmtime_r rpl_gmtime_r # endif _GL_FUNCDECL_RPL (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # else # if ! @HAVE_DECL_LOCALTIME_R@ _GL_FUNCDECL_SYS (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (gmtime_r, struct tm *, (time_t const *restrict __timer, struct tm *restrict __result)); # endif # if @HAVE_DECL_LOCALTIME_R@ _GL_CXXALIASWARN (gmtime_r); # endif # endif /* Convert TIMER to RESULT, assuming local time and UTC respectively. See and . */ # if @GNULIB_LOCALTIME@ || @REPLACE_LOCALTIME@ # if @REPLACE_LOCALTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef localtime # define localtime rpl_localtime # endif _GL_FUNCDECL_RPL (localtime, struct tm *, (time_t const *__timer) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (localtime, struct tm *, (time_t const *__timer)); # else _GL_CXXALIAS_SYS (localtime, struct tm *, (time_t const *__timer)); # endif _GL_CXXALIASWARN (localtime); # endif # if 0 || @REPLACE_GMTIME@ # if @REPLACE_GMTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gmtime # define gmtime rpl_gmtime # endif _GL_FUNCDECL_RPL (gmtime, struct tm *, (time_t const *__timer) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (gmtime, struct tm *, (time_t const *__timer)); # else _GL_CXXALIAS_SYS (gmtime, struct tm *, (time_t const *__timer)); # endif _GL_CXXALIASWARN (gmtime); # endif /* Parse BUF as a timestamp, assuming FORMAT specifies its layout, and store the resulting broken-down time into TM. See . */ # if @GNULIB_STRPTIME@ # if ! @HAVE_STRPTIME@ _GL_FUNCDECL_SYS (strptime, char *, (char const *restrict __buf, char const *restrict __format, struct tm *restrict __tm) _GL_ARG_NONNULL ((1, 2, 3))); # endif _GL_CXXALIAS_SYS (strptime, char *, (char const *restrict __buf, char const *restrict __format, struct tm *restrict __tm)); _GL_CXXALIASWARN (strptime); # endif /* Convert *TP to a date and time string. See . */ # if @GNULIB_CTIME@ # if @REPLACE_CTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define ctime rpl_ctime # endif _GL_FUNCDECL_RPL (ctime, char *, (time_t const *__tp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (ctime, char *, (time_t const *__tp)); # else _GL_CXXALIAS_SYS (ctime, char *, (time_t const *__tp)); # endif _GL_CXXALIASWARN (ctime); # endif /* Convert *TP to a date and time string. See . */ # if @GNULIB_STRFTIME@ # if @REPLACE_STRFTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strftime rpl_strftime # endif _GL_FUNCDECL_RPL (strftime, size_t, (char *__buf, size_t __bufsize, const char *__fmt, const struct tm *__tp) _GL_ARG_NONNULL ((1, 3, 4))); _GL_CXXALIAS_RPL (strftime, size_t, (char *__buf, size_t __bufsize, const char *__fmt, const struct tm *__tp)); # else _GL_CXXALIAS_SYS (strftime, size_t, (char *__buf, size_t __bufsize, const char *__fmt, const struct tm *__tp)); # endif _GL_CXXALIASWARN (strftime); # endif # if defined _GNU_SOURCE && @GNULIB_TIME_RZ@ && ! @HAVE_TIMEZONE_T@ typedef struct tm_zone *timezone_t; _GL_FUNCDECL_SYS (tzalloc, timezone_t, (char const *__name)); _GL_CXXALIAS_SYS (tzalloc, timezone_t, (char const *__name)); _GL_FUNCDECL_SYS (tzfree, void, (timezone_t __tz)); _GL_CXXALIAS_SYS (tzfree, void, (timezone_t __tz)); _GL_FUNCDECL_SYS (localtime_rz, struct tm *, (timezone_t __tz, time_t const *restrict __timer, struct tm *restrict __result) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_SYS (localtime_rz, struct tm *, (timezone_t __tz, time_t const *restrict __timer, struct tm *restrict __result)); _GL_FUNCDECL_SYS (mktime_z, time_t, (timezone_t __tz, struct tm *restrict __result) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_SYS (mktime_z, time_t, (timezone_t __tz, struct tm *restrict __result)); # endif /* Convert TM to a time_t value, assuming UTC. */ # if @GNULIB_TIMEGM@ # if @REPLACE_TIMEGM@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef timegm # define timegm rpl_timegm # endif _GL_FUNCDECL_RPL (timegm, time_t, (struct tm *__tm) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (timegm, time_t, (struct tm *__tm)); # else # if ! @HAVE_TIMEGM@ _GL_FUNCDECL_SYS (timegm, time_t, (struct tm *__tm) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (timegm, time_t, (struct tm *__tm)); # endif _GL_CXXALIASWARN (timegm); # endif /* Encourage applications to avoid unsafe functions that can overrun buffers when given outlandish struct tm values. Portable applications should use strftime (or even sprintf) instead. */ # if defined GNULIB_POSIXCHECK # undef asctime _GL_WARN_ON_USE (asctime, "asctime can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif # if defined GNULIB_POSIXCHECK # undef asctime_r _GL_WARN_ON_USE (asctime, "asctime_r can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif # if defined GNULIB_POSIXCHECK # undef ctime _GL_WARN_ON_USE (asctime, "ctime can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif # if defined GNULIB_POSIXCHECK # undef ctime_r _GL_WARN_ON_USE (asctime, "ctime_r can overrun buffers in some cases - " "better use strftime (or even sprintf) instead"); # endif #endif gnuastro-0.5/bootstrapped/tests/test-init.sh0000755000175000017500000000463413217200023016265 00000000000000#!/bin/sh # Unit tests for init.sh # Copyright (C) 2011-2017 Free Software Foundation, Inc. # This file is part of the GNUlib Library. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . */ : ${srcdir=.} . "$srcdir/init.sh"; path_prepend_ . fail=0 test_compare() { touch empty || fail=1 echo xyz > in || fail=1 compare /dev/null /dev/null >out 2>err || fail=1 test -s out && fail_ "out not empty: $(cat out)" # "err" should be empty, too, but has "set -x" output when VERBOSE=yes case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare /dev/null empty >out 2>err || fail=1 test -s out && fail_ "out not empty: $(cat out)" case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare in in >out 2>err || fail=1 test -s out && fail_ "out not empty: $(cat out)" case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare /dev/null in >out 2>err && fail=1 cat <<\EOF > exp diff -u /dev/null in --- /dev/null 1970-01-01 +++ in 1970-01-01 +xyz EOF compare exp out || fail=1 case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac compare empty in >out 2>err && fail=1 # Compare against expected output only if compare is using diff -u. if grep @ out >/dev/null; then # Remove the TAB-date suffix on each --- and +++ line, # for both the expected and the actual output files. # Also remove the @@ line, since Solaris 5.10 and GNU diff formats differ: # -@@ -0,0 +1 @@ # +@@ -1,0 +1,1 @@ # Also, remove space after leading '+', since AIX 7.1 diff outputs a space. sed 's/ .*//;/^@@/d;s/^+ /+/' out > k && mv k out cat <<\EOF > exp --- empty +++ in +xyz EOF compare exp out || fail=1 fi case $- in *x*) ;; *) test -s err && fail_ "err not empty: $(cat err)";; esac } test_compare Exit $fail gnuastro-0.5/bootstrapped/tests/init.sh0000644000175000017500000005022513217200022015301 00000000000000# source this file; set up for tests # Copyright (C) 2009-2017 Free Software Foundation, Inc. # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation, either version 3 of the License, or # (at your option) any later version. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see . # Using this file in a test # ========================= # # The typical skeleton of a test looks like this: # # #!/bin/sh # . "${srcdir=.}/init.sh"; path_prepend_ . # Execute some commands. # Note that these commands are executed in a subdirectory, therefore you # need to prepend "../" to relative filenames in the build directory. # Note that the "path_prepend_ ." is useful only if the body of your # test invokes programs residing in the initial directory. # For example, if the programs you want to test are in src/, and this test # script is named tests/test-1, then you would use "path_prepend_ ../src", # or perhaps export PATH='$(abs_top_builddir)/src$(PATH_SEPARATOR)'"$$PATH" # to all tests via automake's TESTS_ENVIRONMENT. # Set the exit code 0 for success, 77 for skipped, or 1 or other for failure. # Use the skip_ and fail_ functions to print a diagnostic and then exit # with the corresponding exit code. # Exit $? # Executing a test that uses this file # ==================================== # # Running a single test: # $ make check TESTS=test-foo.sh # # Running a single test, with verbose output: # $ make check TESTS=test-foo.sh VERBOSE=yes # # Running a single test, keeping the temporary directory: # $ make check TESTS=test-foo.sh KEEP=yes # # Running a single test, with single-stepping: # 1. Go into a sub-shell: # $ bash # 2. Set relevant environment variables from TESTS_ENVIRONMENT in the # Makefile: # $ export srcdir=../../tests # this is an example # 3. Execute the commands from the test, copy&pasting them one by one: # $ . "$srcdir/init.sh"; path_prepend_ . # ... # 4. Finally # $ exit ME_=`expr "./$0" : '.*/\(.*\)$'` # Prepare PATH_SEPARATOR. # The user is always right. if test "${PATH_SEPARATOR+set}" != set; then # Determine PATH_SEPARATOR by trying to find /bin/sh in a PATH which # contains only /bin. Note that ksh looks also at the FPATH variable, # so we have to set that as well for the test. PATH_SEPARATOR=: (PATH='/bin;/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 \ && { (PATH='/bin:/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 \ || PATH_SEPARATOR=';' } fi # We use a trap below for cleanup. This requires us to go through # hoops to get the right exit status transported through the handler. # So use 'Exit STATUS' instead of 'exit STATUS' inside of the tests. # Turn off errexit here so that we don't trip the bug with OSF1/Tru64 # sh inside this function. Exit () { set +e; (exit $1); exit $1; } # Print warnings (e.g., about skipped and failed tests) to this file number. # Override by defining to say, 9, in init.cfg, and putting say, # export ...ENVVAR_SETTINGS...; $(SHELL) 9>&2 # in the definition of TESTS_ENVIRONMENT in your tests/Makefile.am file. # This is useful when using automake's parallel tests mode, to print # the reason for skip/failure to console, rather than to the .log files. : ${stderr_fileno_=2} # Note that correct expansion of "$*" depends on IFS starting with ' '. # Always write the full diagnostic to stderr. # When stderr_fileno_ is not 2, also emit the first line of the # diagnostic to that file descriptor. warn_ () { # If IFS does not start with ' ', set it and emit the warning in a subshell. case $IFS in ' '*) printf '%s\n' "$*" >&2 test $stderr_fileno_ = 2 \ || { printf '%s\n' "$*" | sed 1q >&$stderr_fileno_ ; } ;; *) (IFS=' '; warn_ "$@");; esac } fail_ () { warn_ "$ME_: failed test: $@"; Exit 1; } skip_ () { warn_ "$ME_: skipped test: $@"; Exit 77; } fatal_ () { warn_ "$ME_: hard error: $@"; Exit 99; } framework_failure_ () { warn_ "$ME_: set-up failure: $@"; Exit 99; } # This is used to simplify checking of the return value # which is useful when ensuring a command fails as desired. # I.e., just doing `command ... &&fail=1` will not catch # a segfault in command for example. With this helper you # instead check an explicit exit code like # returns_ 1 command ... || fail returns_ () { # Disable tracing so it doesn't interfere with stderr of the wrapped command { set +x; } 2>/dev/null local exp_exit="$1" shift "$@" test $? -eq $exp_exit && ret_=0 || ret_=1 if test "$VERBOSE" = yes && test "$gl_set_x_corrupts_stderr_" = false; then set -x fi { return $ret_; } 2>/dev/null } # Sanitize this shell to POSIX mode, if possible. DUALCASE=1; export DUALCASE if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST else case `(set -o) 2>/dev/null` in *posix*) set -o posix ;; esac fi # We require $(...) support unconditionally. # We require non-surprising "local" semantics (this eliminates dash). # This takes the admittedly draconian step of eliminating dash, because the # assignment tab=$(printf '\t') works fine, yet preceding it with "local " # transforms it into an assignment that sets the variable to the empty string. # That is too counter-intuitive, and can lead to subtle run-time malfunction. # The example below is less subtle in that with dash, it evokes the run-time # exception "dash: 1: local: 1: bad variable name". # We require a few additional shell features only when $EXEEXT is nonempty, # in order to support automatic $EXEEXT emulation: # - hyphen-containing alias names # - we prefer to use ${var#...} substitution, rather than having # to work around lack of support for that feature. # The following code attempts to find a shell with support for these features. # If the current shell passes the test, we're done. Otherwise, test other # shells until we find one that passes. If one is found, re-exec it. # If no acceptable shell is found, skip the current test. # # The "...set -x; P=1 true 2>err..." test is to disqualify any shell that # emits "P=1" into err, as /bin/sh from SunOS 5.11 and OpenBSD 4.7 do. # # Use "9" to indicate success (rather than 0), in case some shell acts # like Solaris 10's /bin/sh but exits successfully instead of with status 2. # Eval this code in a subshell to determine a shell's suitability. # 10 - passes all tests; ok to use # 9 - ok, but enabling "set -x" corrupts app stderr; prefer higher score # ? - not ok gl_shell_test_script_=' test $(echo y) = y || exit 1 f_local_() { local v=1; }; f_local_ || exit 1 f_dash_local_fail_() { local t=$(printf " 1"); }; f_dash_local_fail_ score_=10 if test "$VERBOSE" = yes; then test -n "$( (exec 3>&1; set -x; P=1 true 2>&3) 2> /dev/null)" && score_=9 fi test -z "$EXEEXT" && exit $score_ shopt -s expand_aliases alias a-b="echo zoo" v=abx test ${v%x} = ab \ && test ${v#a} = bx \ && test $(a-b) = zoo \ && exit $score_ ' if test "x$1" = "x--no-reexec"; then shift else # Assume a working shell. Export to subshells (setup_ needs this). gl_set_x_corrupts_stderr_=false export gl_set_x_corrupts_stderr_ # Record the first marginally acceptable shell. marginal_= # Search for a shell that meets our requirements. for re_shell_ in __current__ "${CONFIG_SHELL:-no_shell}" \ /bin/sh bash dash zsh pdksh fail do test "$re_shell_" = no_shell && continue # If we've made it all the way to the sentinel, "fail" without # finding even a marginal shell, skip this test. if test "$re_shell_" = fail; then test -z "$marginal_" && skip_ failed to find an adequate shell re_shell_=$marginal_ break fi # When testing the current shell, simply "eval" the test code. # Otherwise, run it via $re_shell_ -c ... if test "$re_shell_" = __current__; then # 'eval'ing this code makes Solaris 10's /bin/sh exit with # $? set to 2. It does not evaluate any of the code after the # "unexpected" first '('. Thus, we must run it in a subshell. ( eval "$gl_shell_test_script_" ) > /dev/null 2>&1 else "$re_shell_" -c "$gl_shell_test_script_" 2>/dev/null fi st_=$? # $re_shell_ works just fine. Use it. if test $st_ = 10; then gl_set_x_corrupts_stderr_=false break fi # If this is our first marginally acceptable shell, remember it. if test "$st_:$marginal_" = 9: ; then marginal_="$re_shell_" gl_set_x_corrupts_stderr_=true fi done if test "$re_shell_" != __current__; then # Found a usable shell. Preserve -v and -x. case $- in *v*x* | *x*v*) opts_=-vx ;; *v*) opts_=-v ;; *x*) opts_=-x ;; *) opts_= ;; esac re_shell=$re_shell_ export re_shell exec "$re_shell_" $opts_ "$0" --no-reexec "$@" echo "$ME_: exec failed" 1>&2 exit 127 fi fi # If this is bash, turn off all aliases. test -n "$BASH_VERSION" && unalias -a # Note that when supporting $EXEEXT (transparently mapping from PROG_NAME to # PROG_NAME.exe), we want to support hyphen-containing names like test-acos. # That is part of the shell-selection test above. Why use aliases rather # than functions? Because support for hyphen-containing aliases is more # widespread than that for hyphen-containing function names. test -n "$EXEEXT" && test -n "$BASH_VERSION" && shopt -s expand_aliases # Enable glibc's malloc-perturbing option. # This is useful for exposing code that depends on the fact that # malloc-related functions often return memory that is mostly zeroed. # If you have the time and cycles, use valgrind to do an even better job. : ${MALLOC_PERTURB_=87} export MALLOC_PERTURB_ # This is a stub function that is run upon trap (upon regular exit and # interrupt). Override it with a per-test function, e.g., to unmount # a partition, or to undo any other global state changes. cleanup_ () { :; } # Emit a header similar to that from diff -u; Print the simulated "diff" # command so that the order of arguments is clear. Don't bother with @@ lines. emit_diff_u_header_ () { printf '%s\n' "diff -u $*" \ "--- $1 1970-01-01" \ "+++ $2 1970-01-01" } # Arrange not to let diff or cmp operate on /dev/null, # since on some systems (at least OSF/1 5.1), that doesn't work. # When there are not two arguments, or no argument is /dev/null, return 2. # When one argument is /dev/null and the other is not empty, # cat the nonempty file to stderr and return 1. # Otherwise, return 0. compare_dev_null_ () { test $# = 2 || return 2 if test "x$1" = x/dev/null; then test -s "$2" || return 0 emit_diff_u_header_ "$@"; sed 's/^/+/' "$2" return 1 fi if test "x$2" = x/dev/null; then test -s "$1" || return 0 emit_diff_u_header_ "$@"; sed 's/^/-/' "$1" return 1 fi return 2 } for diff_opt_ in -u -U3 -c '' no; do test "$diff_opt_" != no && diff_out_=`exec 2>/dev/null; diff $diff_opt_ "$0" "$0" < /dev/null` && break done if test "$diff_opt_" != no; then if test -z "$diff_out_"; then compare_ () { diff $diff_opt_ "$@"; } else compare_ () { # If no differences were found, AIX and HP-UX 'diff' produce output # like "No differences encountered". Hide this output. diff $diff_opt_ "$@" > diff.out diff_status_=$? test $diff_status_ -eq 0 || cat diff.out || diff_status_=2 rm -f diff.out || diff_status_=2 return $diff_status_ } fi elif cmp -s /dev/null /dev/null 2>/dev/null; then compare_ () { cmp -s "$@"; } else compare_ () { cmp "$@"; } fi # Usage: compare EXPECTED ACTUAL # # Given compare_dev_null_'s preprocessing, defer to compare_ if 2 or more. # Otherwise, propagate $? to caller: any diffs have already been printed. compare () { # This looks like it can be factored to use a simple "case $?" # after unchecked compare_dev_null_ invocation, but that would # fail in a "set -e" environment. if compare_dev_null_ "$@"; then return 0 else case $? in 1) return 1;; *) compare_ "$@";; esac fi } # An arbitrary prefix to help distinguish test directories. testdir_prefix_ () { printf gt; } # Run the user-overridable cleanup_ function, remove the temporary # directory and exit with the incoming value of $?. remove_tmp_ () { __st=$? cleanup_ if test "$KEEP" = yes; then echo "Not removing temporary directory $test_dir_" else # cd out of the directory we're about to remove cd "$initial_cwd_" || cd / || cd /tmp chmod -R u+rwx "$test_dir_" # If removal fails and exit status was to be 0, then change it to 1. rm -rf "$test_dir_" || { test $__st = 0 && __st=1; } fi exit $__st } # Given a directory name, DIR, if every entry in it that matches *.exe # contains only the specified bytes (see the case stmt below), then print # a space-separated list of those names and return 0. Otherwise, don't # print anything and return 1. Naming constraints apply also to DIR. find_exe_basenames_ () { feb_dir_=$1 feb_fail_=0 feb_result_= feb_sp_= for feb_file_ in $feb_dir_/*.exe; do # If there was no *.exe file, or there existed a file named "*.exe" that # was deleted between the above glob expansion and the existence test # below, just skip it. test "x$feb_file_" = "x$feb_dir_/*.exe" && test ! -f "$feb_file_" \ && continue # Exempt [.exe, since we can't create a function by that name, yet # we can't invoke [ by PATH search anyways due to shell builtins. test "x$feb_file_" = "x$feb_dir_/[.exe" && continue case $feb_file_ in *[!-a-zA-Z/0-9_.+]*) feb_fail_=1; break;; *) # Remove leading file name components as well as the .exe suffix. feb_file_=${feb_file_##*/} feb_file_=${feb_file_%.exe} feb_result_="$feb_result_$feb_sp_$feb_file_";; esac feb_sp_=' ' done test $feb_fail_ = 0 && printf %s "$feb_result_" return $feb_fail_ } # Consider the files in directory, $1. # For each file name of the form PROG.exe, create an alias named # PROG that simply invokes PROG.exe, then return 0. If any selected # file name or the directory name, $1, contains an unexpected character, # define no alias and return 1. create_exe_shims_ () { case $EXEEXT in '') return 0 ;; .exe) ;; *) echo "$0: unexpected \$EXEEXT value: $EXEEXT" 1>&2; return 1 ;; esac base_names_=`find_exe_basenames_ $1` \ || { echo "$0 (exe_shim): skipping directory: $1" 1>&2; return 0; } if test -n "$base_names_"; then for base_ in $base_names_; do alias "$base_"="$base_$EXEEXT" done fi return 0 } # Use this function to prepend to PATH an absolute name for each # specified, possibly-$initial_cwd_-relative, directory. path_prepend_ () { while test $# != 0; do path_dir_=$1 case $path_dir_ in '') fail_ "invalid path dir: '$1'";; /* | ?:*) abs_path_dir_=$path_dir_;; *) abs_path_dir_=$initial_cwd_/$path_dir_;; esac case $abs_path_dir_ in *$PATH_SEPARATOR*) fail_ "invalid path dir: '$abs_path_dir_'";; esac PATH="$abs_path_dir_$PATH_SEPARATOR$PATH" # Create an alias, FOO, for each FOO.exe in this directory. create_exe_shims_ "$abs_path_dir_" \ || fail_ "something failed (above): $abs_path_dir_" shift done export PATH } setup_ () { if test "$VERBOSE" = yes; then # Test whether set -x may cause the selected shell to corrupt an # application's stderr. Many do, including zsh-4.3.10 and the /bin/sh # from SunOS 5.11, OpenBSD 4.7 and Irix 5.x and 6.5. # If enabling verbose output this way would cause trouble, simply # issue a warning and refrain. if $gl_set_x_corrupts_stderr_; then warn_ "using SHELL=$SHELL with 'set -x' corrupts stderr" else set -x fi fi initial_cwd_=$PWD pfx_=`testdir_prefix_` test_dir_=`mktempd_ "$initial_cwd_" "$pfx_-$ME_.XXXX"` \ || fail_ "failed to create temporary directory in $initial_cwd_" cd "$test_dir_" || fail_ "failed to cd to temporary directory" # As autoconf-generated configure scripts do, ensure that IFS # is defined initially, so that saving and restoring $IFS works. gl_init_sh_nl_=' ' IFS=" "" $gl_init_sh_nl_" # This trap statement, along with a trap on 0 below, ensure that the # temporary directory, $test_dir_, is removed upon exit as well as # upon receipt of any of the listed signals. for sig_ in 1 2 3 13 15; do eval "trap 'Exit $(expr $sig_ + 128)' $sig_" done } # Create a temporary directory, much like mktemp -d does. # Written by Jim Meyering. # # Usage: mktempd_ /tmp phoey.XXXXXXXXXX # # First, try to use the mktemp program. # Failing that, we'll roll our own mktemp-like function: # - try to get random bytes from /dev/urandom # - failing that, generate output from a combination of quickly-varying # sources and gzip. Ignore non-varying gzip header, and extract # "random" bits from there. # - given those bits, map to file-name bytes using tr, and try to create # the desired directory. # - make only $MAX_TRIES_ attempts # Helper function. Print $N pseudo-random bytes from a-zA-Z0-9. rand_bytes_ () { n_=$1 # Maybe try openssl rand -base64 $n_prime_|tr '+/=\012' abcd first? # But if they have openssl, they probably have mktemp, too. chars_=abcdefghijklmnopqrstuvwxyzABCDEFGHIJKLMNOPQRSTUVWXYZ0123456789 dev_rand_=/dev/urandom if test -r "$dev_rand_"; then # Note: 256-length($chars_) == 194; 3 copies of $chars_ is 186 + 8 = 194. dd ibs=$n_ count=1 if=$dev_rand_ 2>/dev/null \ | LC_ALL=C tr -c $chars_ 01234567$chars_$chars_$chars_ return fi n_plus_50_=`expr $n_ + 50` cmds_='date; date +%N; free; who -a; w; ps auxww; ps ef; netstat -n' data_=` (eval "$cmds_") 2>&1 | gzip ` # Ensure that $data_ has length at least 50+$n_ while :; do len_=`echo "$data_"|wc -c` test $n_plus_50_ -le $len_ && break; data_=` (echo "$data_"; eval "$cmds_") 2>&1 | gzip ` done echo "$data_" \ | dd bs=1 skip=50 count=$n_ 2>/dev/null \ | LC_ALL=C tr -c $chars_ 01234567$chars_$chars_$chars_ } mktempd_ () { case $# in 2);; *) fail_ "Usage: mktempd_ DIR TEMPLATE";; esac destdir_=$1 template_=$2 MAX_TRIES_=4 # Disallow any trailing slash on specified destdir: # it would subvert the post-mktemp "case"-based destdir test. case $destdir_ in / | //) destdir_slash_=$destdir;; */) fail_ "invalid destination dir: remove trailing slash(es)";; *) destdir_slash_=$destdir_/;; esac case $template_ in *XXXX) ;; *) fail_ \ "invalid template: $template_ (must have a suffix of at least 4 X's)";; esac # First, try to use mktemp. d=`unset TMPDIR; { mktemp -d -t -p "$destdir_" "$template_"; } 2>/dev/null` && # The resulting name must be in the specified directory. case $d in "$destdir_slash_"*) :;; *) false;; esac && # It must have created the directory. test -d "$d" && # It must have 0700 permissions. Handle sticky "S" bits. perms=`ls -dgo "$d" 2>/dev/null` && case $perms in drwx--[-S]---*) :;; *) false;; esac && { echo "$d" return } # If we reach this point, we'll have to create a directory manually. # Get a copy of the template without its suffix of X's. base_template_=`echo "$template_"|sed 's/XX*$//'` # Calculate how many X's we've just removed. template_length_=`echo "$template_" | wc -c` nx_=`echo "$base_template_" | wc -c` nx_=`expr $template_length_ - $nx_` err_= i_=1 while :; do X_=`rand_bytes_ $nx_` candidate_dir_="$destdir_slash_$base_template_$X_" err_=`mkdir -m 0700 "$candidate_dir_" 2>&1` \ && { echo "$candidate_dir_"; return; } test $MAX_TRIES_ -le $i_ && break; i_=`expr $i_ + 1` done fail_ "$err_" } # If you want to override the testdir_prefix_ function, # or to add more utility functions, use this file. test -f "$srcdir/init.cfg" \ && . "$srcdir/init.cfg" setup_ "$@" # This trap is here, rather than in the setup_ function, because some # shells run the exit trap at shell function exit, rather than script exit. trap remove_tmp_ 0 gnuastro-0.5/bootstrapped/tests/sys_uio.in.h0000644000175000017500000000317513217200023016255 00000000000000/* Substitute for . Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ # if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ # endif @PRAGMA_COLUMNS@ #ifndef _@GUARD_PREFIX@_SYS_UIO_H #if @HAVE_SYS_UIO_H@ /* On OpenBSD 4.4, assumes prior inclusion of . */ # include /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_SYS_UIO_H@ #endif #ifndef _@GUARD_PREFIX@_SYS_UIO_H #define _@GUARD_PREFIX@_SYS_UIO_H #if !@HAVE_SYS_UIO_H@ /* A platform that lacks . */ /* Get 'size_t' and 'ssize_t'. */ # include # ifdef __cplusplus extern "C" { # endif # if !GNULIB_defined_struct_iovec /* All known platforms that lack also lack any declaration of struct iovec in any other header. */ struct iovec { void *iov_base; size_t iov_len; }; # define GNULIB_defined_struct_iovec 1 # endif # ifdef __cplusplus } # endif #endif #endif /* _@GUARD_PREFIX@_SYS_UIO_H */ #endif /* _@GUARD_PREFIX@_SYS_UIO_H */ gnuastro-0.5/bootstrapped/tests/sys_time.in.h0000644000175000017500000001721613217200023016420 00000000000000/* Provide a more complete sys/time.h. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Paul Eggert. */ #ifndef _@GUARD_PREFIX@_SYS_TIME_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* On Cygwin and on many BSDish systems, includes itself recursively via . Simply delegate to the system's header in this case; it is a no-op. Without this extra ifdef, the C++ gettimeofday declaration below would be a forward declaration in gnulib's nested . */ #if defined _CYGWIN_SYS_TIME_H || defined _SYS_TIME_H || defined _SYS_TIME_H_ # @INCLUDE_NEXT@ @NEXT_SYS_TIME_H@ #else /* The include_next requires a split double-inclusion guard. */ #if @HAVE_SYS_TIME_H@ # @INCLUDE_NEXT@ @NEXT_SYS_TIME_H@ #endif #ifndef _@GUARD_PREFIX@_SYS_TIME_H #define _@GUARD_PREFIX@_SYS_TIME_H #if ! @HAVE_SYS_TIME_H@ # include #endif /* On native Windows with MSVC, get the 'struct timeval' type. Also, on native Windows with a 64-bit time_t, where we are overriding the 'struct timeval' type, get all declarations of system functions whose signature contains 'struct timeval'. */ #if (defined _MSC_VER || @REPLACE_STRUCT_TIMEVAL@) && @HAVE_WINSOCK2_H@ && !defined _GL_INCLUDING_WINSOCK2_H # define _GL_INCLUDING_WINSOCK2_H # include # undef _GL_INCLUDING_WINSOCK2_H #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #ifdef __cplusplus extern "C" { #endif #if !@HAVE_STRUCT_TIMEVAL@ || @REPLACE_STRUCT_TIMEVAL@ # if @REPLACE_STRUCT_TIMEVAL@ # define timeval rpl_timeval # endif # if !GNULIB_defined_struct_timeval struct timeval { time_t tv_sec; long int tv_usec; }; # define GNULIB_defined_struct_timeval 1 # endif #endif #ifdef __cplusplus } #endif #if @GNULIB_GETTIMEOFDAY@ # if @REPLACE_GETTIMEOFDAY@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gettimeofday # define gettimeofday rpl_gettimeofday # endif _GL_FUNCDECL_RPL (gettimeofday, int, (struct timeval *restrict, void *restrict) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (gettimeofday, int, (struct timeval *restrict, void *restrict)); # else # if !@HAVE_GETTIMEOFDAY@ _GL_FUNCDECL_SYS (gettimeofday, int, (struct timeval *restrict, void *restrict) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on glibc systems, by default, the second argument is struct timezone *. */ _GL_CXXALIAS_SYS_CAST (gettimeofday, int, (struct timeval *restrict, void *restrict)); # endif _GL_CXXALIASWARN (gettimeofday); # if defined __cplusplus && defined GNULIB_NAMESPACE namespace GNULIB_NAMESPACE { typedef ::timeval #undef timeval timeval; } # endif #elif defined GNULIB_POSIXCHECK # undef gettimeofday # if HAVE_RAW_DECL_GETTIMEOFDAY _GL_WARN_ON_USE (gettimeofday, "gettimeofday is unportable - " "use gnulib module gettimeofday for portability"); # endif #endif /* Hide some function declarations from . */ #if defined _MSC_VER && @HAVE_WINSOCK2_H@ # if !defined _@GUARD_PREFIX@_UNISTD_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef close # define close close_used_without_including_unistd_h # else _GL_WARN_ON_USE (close, "close() used without including "); # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gethostname # define gethostname gethostname_used_without_including_unistd_h # else _GL_WARN_ON_USE (gethostname, "gethostname() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SOCKET_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef socket # define socket socket_used_without_including_sys_socket_h # undef connect # define connect connect_used_without_including_sys_socket_h # undef accept # define accept accept_used_without_including_sys_socket_h # undef bind # define bind bind_used_without_including_sys_socket_h # undef getpeername # define getpeername getpeername_used_without_including_sys_socket_h # undef getsockname # define getsockname getsockname_used_without_including_sys_socket_h # undef getsockopt # define getsockopt getsockopt_used_without_including_sys_socket_h # undef listen # define listen listen_used_without_including_sys_socket_h # undef recv # define recv recv_used_without_including_sys_socket_h # undef send # define send send_used_without_including_sys_socket_h # undef recvfrom # define recvfrom recvfrom_used_without_including_sys_socket_h # undef sendto # define sendto sendto_used_without_including_sys_socket_h # undef setsockopt # define setsockopt setsockopt_used_without_including_sys_socket_h # undef shutdown # define shutdown shutdown_used_without_including_sys_socket_h # else _GL_WARN_ON_USE (socket, "socket() used without including "); _GL_WARN_ON_USE (connect, "connect() used without including "); _GL_WARN_ON_USE (accept, "accept() used without including "); _GL_WARN_ON_USE (bind, "bind() used without including "); _GL_WARN_ON_USE (getpeername, "getpeername() used without including "); _GL_WARN_ON_USE (getsockname, "getsockname() used without including "); _GL_WARN_ON_USE (getsockopt, "getsockopt() used without including "); _GL_WARN_ON_USE (listen, "listen() used without including "); _GL_WARN_ON_USE (recv, "recv() used without including "); _GL_WARN_ON_USE (send, "send() used without including "); _GL_WARN_ON_USE (recvfrom, "recvfrom() used without including "); _GL_WARN_ON_USE (sendto, "sendto() used without including "); _GL_WARN_ON_USE (setsockopt, "setsockopt() used without including "); _GL_WARN_ON_USE (shutdown, "shutdown() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SELECT_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef select # define select select_used_without_including_sys_select_h # else _GL_WARN_ON_USE (select, "select() used without including "); # endif # endif #endif #endif /* _@GUARD_PREFIX@_SYS_TIME_H */ #endif /* _CYGWIN_SYS_TIME_H */ #endif /* _@GUARD_PREFIX@_SYS_TIME_H */ gnuastro-0.5/bootstrapped/tests/sys_stat.in.h0000644000175000017500000005370213217200023016435 00000000000000/* Provide a more complete sys/stat.h header file. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake, Paul Eggert, and Jim Meyering. */ /* This file is supposed to be used on platforms where is incomplete. It is intended to provide definitions and prototypes needed by an application. Start with what the system provides. */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_system_sys_stat_h /* Special invocation convention. */ #@INCLUDE_NEXT@ @NEXT_SYS_STAT_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_SYS_STAT_H /* Get nlink_t. May also define off_t to a 64-bit type on native Windows. */ #include /* Get struct timespec. */ #include /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_SYS_STAT_H@ #ifndef _@GUARD_PREFIX@_SYS_STAT_H #define _@GUARD_PREFIX@_SYS_STAT_H /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Before doing "#define mkdir rpl_mkdir" below, we need to include all headers that may declare mkdir(). Native Windows platforms declare mkdir in and/or , not in . */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include /* mingw32, mingw64 */ # include /* mingw64, MSVC 9 */ #endif /* Native Windows platforms declare umask() in . */ #if 0 && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif /* Large File Support on native Windows. */ #if @WINDOWS_64_BIT_ST_SIZE@ # define stat _stati64 #endif /* Optionally, override 'struct stat' on native Windows. */ #if @GNULIB_OVERRIDES_STRUCT_STAT@ # undef stat # if @GNULIB_STAT@ # define stat rpl_stat # else /* Provoke a clear link error if stat() is used as a function and module 'stat' is not in use. */ # define stat stat_used_without_requesting_gnulib_module_stat # endif # if !GNULIB_defined_struct_stat struct stat { dev_t st_dev; ino_t st_ino; mode_t st_mode; nlink_t st_nlink; # if 0 uid_t st_uid; # else /* uid_t is not defined by default on native Windows. */ short st_uid; # endif # if 0 gid_t st_gid; # else /* gid_t is not defined by default on native Windows. */ short st_gid; # endif dev_t st_rdev; off_t st_size; # if 0 blksize_t st_blksize; blkcnt_t st_blocks; # endif # if @WINDOWS_STAT_TIMESPEC@ struct timespec st_atim; struct timespec st_mtim; struct timespec st_ctim; # else time_t st_atime; time_t st_mtime; time_t st_ctime; # endif }; # if @WINDOWS_STAT_TIMESPEC@ # define st_atime st_atim.tv_sec # define st_mtime st_mtim.tv_sec # define st_ctime st_ctim.tv_sec /* Indicator, for gnulib internal purposes. */ # define _GL_WINDOWS_STAT_TIMESPEC 1 # endif # define GNULIB_defined_struct_stat 1 # endif /* Other possible values of st_mode. */ # if 0 # define _S_IFBLK 0x6000 # endif # if 0 # define _S_IFLNK 0xA000 # endif # if 0 # define _S_IFSOCK 0xC000 # endif #endif #ifndef S_IFIFO # ifdef _S_IFIFO # define S_IFIFO _S_IFIFO # endif #endif #ifndef S_IFMT # define S_IFMT 0170000 #endif #if STAT_MACROS_BROKEN # undef S_ISBLK # undef S_ISCHR # undef S_ISDIR # undef S_ISFIFO # undef S_ISLNK # undef S_ISNAM # undef S_ISMPB # undef S_ISMPC # undef S_ISNWK # undef S_ISREG # undef S_ISSOCK #endif #ifndef S_ISBLK # ifdef S_IFBLK # define S_ISBLK(m) (((m) & S_IFMT) == S_IFBLK) # else # define S_ISBLK(m) 0 # endif #endif #ifndef S_ISCHR # ifdef S_IFCHR # define S_ISCHR(m) (((m) & S_IFMT) == S_IFCHR) # else # define S_ISCHR(m) 0 # endif #endif #ifndef S_ISDIR # ifdef S_IFDIR # define S_ISDIR(m) (((m) & S_IFMT) == S_IFDIR) # else # define S_ISDIR(m) 0 # endif #endif #ifndef S_ISDOOR /* Solaris 2.5 and up */ # define S_ISDOOR(m) 0 #endif #ifndef S_ISFIFO # ifdef S_IFIFO # define S_ISFIFO(m) (((m) & S_IFMT) == S_IFIFO) # else # define S_ISFIFO(m) 0 # endif #endif #ifndef S_ISLNK # ifdef S_IFLNK # define S_ISLNK(m) (((m) & S_IFMT) == S_IFLNK) # else # define S_ISLNK(m) 0 # endif #endif #ifndef S_ISMPB /* V7 */ # ifdef S_IFMPB # define S_ISMPB(m) (((m) & S_IFMT) == S_IFMPB) # define S_ISMPC(m) (((m) & S_IFMT) == S_IFMPC) # else # define S_ISMPB(m) 0 # define S_ISMPC(m) 0 # endif #endif #ifndef S_ISMPX /* AIX */ # define S_ISMPX(m) 0 #endif #ifndef S_ISNAM /* Xenix */ # ifdef S_IFNAM # define S_ISNAM(m) (((m) & S_IFMT) == S_IFNAM) # else # define S_ISNAM(m) 0 # endif #endif #ifndef S_ISNWK /* HP/UX */ # ifdef S_IFNWK # define S_ISNWK(m) (((m) & S_IFMT) == S_IFNWK) # else # define S_ISNWK(m) 0 # endif #endif #ifndef S_ISPORT /* Solaris 10 and up */ # define S_ISPORT(m) 0 #endif #ifndef S_ISREG # ifdef S_IFREG # define S_ISREG(m) (((m) & S_IFMT) == S_IFREG) # else # define S_ISREG(m) 0 # endif #endif #ifndef S_ISSOCK # ifdef S_IFSOCK # define S_ISSOCK(m) (((m) & S_IFMT) == S_IFSOCK) # else # define S_ISSOCK(m) 0 # endif #endif #ifndef S_TYPEISMQ # define S_TYPEISMQ(p) 0 #endif #ifndef S_TYPEISTMO # define S_TYPEISTMO(p) 0 #endif #ifndef S_TYPEISSEM # ifdef S_INSEM # define S_TYPEISSEM(p) (S_ISNAM ((p)->st_mode) && (p)->st_rdev == S_INSEM) # else # define S_TYPEISSEM(p) 0 # endif #endif #ifndef S_TYPEISSHM # ifdef S_INSHD # define S_TYPEISSHM(p) (S_ISNAM ((p)->st_mode) && (p)->st_rdev == S_INSHD) # else # define S_TYPEISSHM(p) 0 # endif #endif /* high performance ("contiguous data") */ #ifndef S_ISCTG # define S_ISCTG(p) 0 #endif /* Cray DMF (data migration facility): off line, with data */ #ifndef S_ISOFD # define S_ISOFD(p) 0 #endif /* Cray DMF (data migration facility): off line, with no data */ #ifndef S_ISOFL # define S_ISOFL(p) 0 #endif /* 4.4BSD whiteout */ #ifndef S_ISWHT # define S_ISWHT(m) 0 #endif /* If any of the following are undefined, define them to their de facto standard values. */ #if !S_ISUID # define S_ISUID 04000 #endif #if !S_ISGID # define S_ISGID 02000 #endif /* S_ISVTX is a common extension to POSIX. */ #ifndef S_ISVTX # define S_ISVTX 01000 #endif #if !S_IRUSR && S_IREAD # define S_IRUSR S_IREAD #endif #if !S_IRUSR # define S_IRUSR 00400 #endif #if !S_IRGRP # define S_IRGRP (S_IRUSR >> 3) #endif #if !S_IROTH # define S_IROTH (S_IRUSR >> 6) #endif #if !S_IWUSR && S_IWRITE # define S_IWUSR S_IWRITE #endif #if !S_IWUSR # define S_IWUSR 00200 #endif #if !S_IWGRP # define S_IWGRP (S_IWUSR >> 3) #endif #if !S_IWOTH # define S_IWOTH (S_IWUSR >> 6) #endif #if !S_IXUSR && S_IEXEC # define S_IXUSR S_IEXEC #endif #if !S_IXUSR # define S_IXUSR 00100 #endif #if !S_IXGRP # define S_IXGRP (S_IXUSR >> 3) #endif #if !S_IXOTH # define S_IXOTH (S_IXUSR >> 6) #endif #if !S_IRWXU # define S_IRWXU (S_IRUSR | S_IWUSR | S_IXUSR) #endif #if !S_IRWXG # define S_IRWXG (S_IRGRP | S_IWGRP | S_IXGRP) #endif #if !S_IRWXO # define S_IRWXO (S_IROTH | S_IWOTH | S_IXOTH) #endif /* S_IXUGO is a common extension to POSIX. */ #if !S_IXUGO # define S_IXUGO (S_IXUSR | S_IXGRP | S_IXOTH) #endif #ifndef S_IRWXUGO # define S_IRWXUGO (S_IRWXU | S_IRWXG | S_IRWXO) #endif /* Macros for futimens and utimensat. */ #ifndef UTIME_NOW # define UTIME_NOW (-1) # define UTIME_OMIT (-2) #endif #if @GNULIB_FCHMODAT@ # if !@HAVE_FCHMODAT@ _GL_FUNCDECL_SYS (fchmodat, int, (int fd, char const *file, mode_t mode, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (fchmodat, int, (int fd, char const *file, mode_t mode, int flag)); _GL_CXXALIASWARN (fchmodat); #elif defined GNULIB_POSIXCHECK # undef fchmodat # if HAVE_RAW_DECL_FCHMODAT _GL_WARN_ON_USE (fchmodat, "fchmodat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_FSTAT@ # if @REPLACE_FSTAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fstat # define fstat rpl_fstat # endif _GL_FUNCDECL_RPL (fstat, int, (int fd, struct stat *buf) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fstat, int, (int fd, struct stat *buf)); # else _GL_CXXALIAS_SYS (fstat, int, (int fd, struct stat *buf)); # endif _GL_CXXALIASWARN (fstat); #elif @GNULIB_OVERRIDES_STRUCT_STAT@ # undef fstat # define fstat fstat_used_without_requesting_gnulib_module_fstat #elif @WINDOWS_64_BIT_ST_SIZE@ /* Above, we define stat to _stati64. */ # define fstat _fstati64 #elif defined GNULIB_POSIXCHECK # undef fstat # if HAVE_RAW_DECL_FSTAT _GL_WARN_ON_USE (fstat, "fstat has portability problems - " "use gnulib module fstat for portability"); # endif #endif #if @GNULIB_FSTATAT@ # if @REPLACE_FSTATAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fstatat # define fstatat rpl_fstatat # endif _GL_FUNCDECL_RPL (fstatat, int, (int fd, char const *name, struct stat *st, int flags) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (fstatat, int, (int fd, char const *name, struct stat *st, int flags)); # else # if !@HAVE_FSTATAT@ _GL_FUNCDECL_SYS (fstatat, int, (int fd, char const *name, struct stat *st, int flags) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (fstatat, int, (int fd, char const *name, struct stat *st, int flags)); # endif _GL_CXXALIASWARN (fstatat); #elif @GNULIB_OVERRIDES_STRUCT_STAT@ # undef fstatat # define fstatat fstatat_used_without_requesting_gnulib_module_fstatat #elif defined GNULIB_POSIXCHECK # undef fstatat # if HAVE_RAW_DECL_FSTATAT _GL_WARN_ON_USE (fstatat, "fstatat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_FUTIMENS@ /* Use the rpl_ prefix also on Solaris <= 9, because on Solaris 9 our futimens implementation relies on futimesat, which on Solaris 10 makes an invocation to futimens that is meant to invoke the libc's futimens(), not gnulib's futimens(). */ # if @REPLACE_FUTIMENS@ || (!@HAVE_FUTIMENS@ && defined __sun) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef futimens # define futimens rpl_futimens # endif _GL_FUNCDECL_RPL (futimens, int, (int fd, struct timespec const times[2])); _GL_CXXALIAS_RPL (futimens, int, (int fd, struct timespec const times[2])); # else # if !@HAVE_FUTIMENS@ _GL_FUNCDECL_SYS (futimens, int, (int fd, struct timespec const times[2])); # endif _GL_CXXALIAS_SYS (futimens, int, (int fd, struct timespec const times[2])); # endif # if @HAVE_FUTIMENS@ _GL_CXXALIASWARN (futimens); # endif #elif defined GNULIB_POSIXCHECK # undef futimens # if HAVE_RAW_DECL_FUTIMENS _GL_WARN_ON_USE (futimens, "futimens is not portable - " "use gnulib module futimens for portability"); # endif #endif #if @GNULIB_LCHMOD@ /* Change the mode of FILENAME to MODE, without dereferencing it if FILENAME denotes a symbolic link. */ # if !@HAVE_LCHMOD@ /* The lchmod replacement follows symbolic links. Callers should take this into account; lchmod should be applied only to arguments that are known to not be symbolic links. On hosts that lack lchmod, this can lead to race conditions between the check and the invocation of lchmod, but we know of no workarounds that are reliable in general. You might try requesting support for lchmod from your operating system supplier. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define lchmod chmod # endif /* Need to cast, because on mingw, the second parameter of chmod is int mode. */ _GL_CXXALIAS_RPL_CAST_1 (lchmod, chmod, int, (const char *filename, mode_t mode)); # else # if 0 /* assume already declared */ _GL_FUNCDECL_SYS (lchmod, int, (const char *filename, mode_t mode) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (lchmod, int, (const char *filename, mode_t mode)); # endif # if @HAVE_LCHMOD@ _GL_CXXALIASWARN (lchmod); # endif #elif defined GNULIB_POSIXCHECK # undef lchmod # if HAVE_RAW_DECL_LCHMOD _GL_WARN_ON_USE (lchmod, "lchmod is unportable - " "use gnulib module lchmod for portability"); # endif #endif #if @GNULIB_LSTAT@ # if ! @HAVE_LSTAT@ /* mingw does not support symlinks, therefore it does not have lstat. But without links, stat does just fine. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define lstat stat # endif _GL_CXXALIAS_RPL_1 (lstat, stat, int, (const char *name, struct stat *buf)); # elif @REPLACE_LSTAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef lstat # define lstat rpl_lstat # endif _GL_FUNCDECL_RPL (lstat, int, (const char *name, struct stat *buf) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (lstat, int, (const char *name, struct stat *buf)); # else _GL_CXXALIAS_SYS (lstat, int, (const char *name, struct stat *buf)); # endif # if @HAVE_LSTAT@ _GL_CXXALIASWARN (lstat); # endif #elif @GNULIB_OVERRIDES_STRUCT_STAT@ # undef lstat # define lstat lstat_used_without_requesting_gnulib_module_lstat #elif defined GNULIB_POSIXCHECK # undef lstat # if HAVE_RAW_DECL_LSTAT _GL_WARN_ON_USE (lstat, "lstat is unportable - " "use gnulib module lstat for portability"); # endif #endif #if @REPLACE_MKDIR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mkdir # define mkdir rpl_mkdir # endif _GL_FUNCDECL_RPL (mkdir, int, (char const *name, mode_t mode) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mkdir, int, (char const *name, mode_t mode)); #else /* mingw's _mkdir() function has 1 argument, but we pass 2 arguments. Additionally, it declares _mkdir (and depending on compile flags, an alias mkdir), only in the nonstandard includes and , which are included above. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # if !GNULIB_defined_rpl_mkdir static int rpl_mkdir (char const *name, mode_t mode) { return _mkdir (name); } # define GNULIB_defined_rpl_mkdir 1 # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mkdir rpl_mkdir # endif _GL_CXXALIAS_RPL (mkdir, int, (char const *name, mode_t mode)); # else _GL_CXXALIAS_SYS (mkdir, int, (char const *name, mode_t mode)); # endif #endif _GL_CXXALIASWARN (mkdir); #if @GNULIB_MKDIRAT@ # if !@HAVE_MKDIRAT@ _GL_FUNCDECL_SYS (mkdirat, int, (int fd, char const *file, mode_t mode) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mkdirat, int, (int fd, char const *file, mode_t mode)); _GL_CXXALIASWARN (mkdirat); #elif defined GNULIB_POSIXCHECK # undef mkdirat # if HAVE_RAW_DECL_MKDIRAT _GL_WARN_ON_USE (mkdirat, "mkdirat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_MKFIFO@ # if @REPLACE_MKFIFO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mkfifo # define mkfifo rpl_mkfifo # endif _GL_FUNCDECL_RPL (mkfifo, int, (char const *file, mode_t mode) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mkfifo, int, (char const *file, mode_t mode)); # else # if !@HAVE_MKFIFO@ _GL_FUNCDECL_SYS (mkfifo, int, (char const *file, mode_t mode) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkfifo, int, (char const *file, mode_t mode)); # endif _GL_CXXALIASWARN (mkfifo); #elif defined GNULIB_POSIXCHECK # undef mkfifo # if HAVE_RAW_DECL_MKFIFO _GL_WARN_ON_USE (mkfifo, "mkfifo is not portable - " "use gnulib module mkfifo for portability"); # endif #endif #if @GNULIB_MKFIFOAT@ # if !@HAVE_MKFIFOAT@ _GL_FUNCDECL_SYS (mkfifoat, int, (int fd, char const *file, mode_t mode) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mkfifoat, int, (int fd, char const *file, mode_t mode)); _GL_CXXALIASWARN (mkfifoat); #elif defined GNULIB_POSIXCHECK # undef mkfifoat # if HAVE_RAW_DECL_MKFIFOAT _GL_WARN_ON_USE (mkfifoat, "mkfifoat is not portable - " "use gnulib module mkfifoat for portability"); # endif #endif #if @GNULIB_MKNOD@ # if @REPLACE_MKNOD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mknod # define mknod rpl_mknod # endif _GL_FUNCDECL_RPL (mknod, int, (char const *file, mode_t mode, dev_t dev) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mknod, int, (char const *file, mode_t mode, dev_t dev)); # else # if !@HAVE_MKNOD@ _GL_FUNCDECL_SYS (mknod, int, (char const *file, mode_t mode, dev_t dev) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on OSF/1 5.1, the third parameter is '...'. */ _GL_CXXALIAS_SYS_CAST (mknod, int, (char const *file, mode_t mode, dev_t dev)); # endif _GL_CXXALIASWARN (mknod); #elif defined GNULIB_POSIXCHECK # undef mknod # if HAVE_RAW_DECL_MKNOD _GL_WARN_ON_USE (mknod, "mknod is not portable - " "use gnulib module mknod for portability"); # endif #endif #if @GNULIB_MKNODAT@ # if !@HAVE_MKNODAT@ _GL_FUNCDECL_SYS (mknodat, int, (int fd, char const *file, mode_t mode, dev_t dev) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mknodat, int, (int fd, char const *file, mode_t mode, dev_t dev)); _GL_CXXALIASWARN (mknodat); #elif defined GNULIB_POSIXCHECK # undef mknodat # if HAVE_RAW_DECL_MKNODAT _GL_WARN_ON_USE (mknodat, "mknodat is not portable - " "use gnulib module mkfifoat for portability"); # endif #endif #if @GNULIB_STAT@ # if @REPLACE_STAT@ # if !@GNULIB_OVERRIDES_STRUCT_STAT@ /* We can't use the object-like #define stat rpl_stat, because of struct stat. This means that rpl_stat will not be used if the user does (stat)(a,b). Oh well. */ # if defined _AIX && defined stat && defined _LARGE_FILES /* With _LARGE_FILES defined, AIX (only) defines stat to stat64, so we have to replace stat64() instead of stat(). */ # undef stat64 # define stat64(name, st) rpl_stat (name, st) # elif @WINDOWS_64_BIT_ST_SIZE@ /* Above, we define stat to _stati64. */ # if defined __MINGW32__ && defined _stati64 # ifndef _USE_32BIT_TIME_T /* The system headers define _stati64 to _stat64. */ # undef _stat64 # define _stat64(name, st) rpl_stat (name, st) # endif # elif defined _MSC_VER && defined _stati64 # ifdef _USE_32BIT_TIME_T /* The system headers define _stati64 to _stat32i64. */ # undef _stat32i64 # define _stat32i64(name, st) rpl_stat (name, st) # else /* The system headers define _stati64 to _stat64. */ # undef _stat64 # define _stat64(name, st) rpl_stat (name, st) # endif # else # undef _stati64 # define _stati64(name, st) rpl_stat (name, st) # endif # elif defined __MINGW32__ && defined stat # ifdef _USE_32BIT_TIME_T /* The system headers define stat to _stat32i64. */ # undef _stat32i64 # define _stat32i64(name, st) rpl_stat (name, st) # else /* The system headers define stat to _stat64. */ # undef _stat64 # define _stat64(name, st) rpl_stat (name, st) # endif # elif defined _MSC_VER && defined stat # ifdef _USE_32BIT_TIME_T /* The system headers define stat to _stat32. */ # undef _stat32 # define _stat32(name, st) rpl_stat (name, st) # else /* The system headers define stat to _stat64i32. */ # undef _stat64i32 # define _stat64i32(name, st) rpl_stat (name, st) # endif # else /* !(_AIX || __MINGW32__ || _MSC_VER) */ # undef stat # define stat(name, st) rpl_stat (name, st) # endif /* !_LARGE_FILES */ # endif /* !@GNULIB_OVERRIDES_STRUCT_STAT@ */ _GL_EXTERN_C int stat (const char *name, struct stat *buf) _GL_ARG_NONNULL ((1, 2)); # endif #elif @GNULIB_OVERRIDES_STRUCT_STAT@ /* see above: #define stat stat_used_without_requesting_gnulib_module_stat */ #elif defined GNULIB_POSIXCHECK # undef stat # if HAVE_RAW_DECL_STAT _GL_WARN_ON_USE (stat, "stat is unportable - " "use gnulib module stat for portability"); # endif #endif #if @GNULIB_UTIMENSAT@ /* Use the rpl_ prefix also on Solaris <= 9, because on Solaris 9 our utimensat implementation relies on futimesat, which on Solaris 10 makes an invocation to utimensat that is meant to invoke the libc's utimensat(), not gnulib's utimensat(). */ # if @REPLACE_UTIMENSAT@ || (!@HAVE_UTIMENSAT@ && defined __sun) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef utimensat # define utimensat rpl_utimensat # endif _GL_FUNCDECL_RPL (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag)); # else # if !@HAVE_UTIMENSAT@ _GL_FUNCDECL_SYS (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (utimensat, int, (int fd, char const *name, struct timespec const times[2], int flag)); # endif # if @HAVE_UTIMENSAT@ _GL_CXXALIASWARN (utimensat); # endif #elif defined GNULIB_POSIXCHECK # undef utimensat # if HAVE_RAW_DECL_UTIMENSAT _GL_WARN_ON_USE (utimensat, "utimensat is not portable - " "use gnulib module utimensat for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_SYS_STAT_H */ #endif /* _@GUARD_PREFIX@_SYS_STAT_H */ #endif gnuastro-0.5/bootstrapped/tests/sys_socket.in.h0000644000175000017500000005533013217200023016751 00000000000000/* Provide a sys/socket header file for systems lacking it (read: MinGW) and for systems where it is incomplete. Copyright (C) 2005-2017 Free Software Foundation, Inc. Written by Simon Josefsson. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file is supposed to be used on platforms that lack , on platforms where cannot be included standalone, and on platforms where does not provide all necessary definitions. It is intended to provide definitions and prototypes needed by an application. */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined _GL_ALREADY_INCLUDING_SYS_SOCKET_H /* Special invocation convention: - On Cygwin 1.5.x we have a sequence of nested includes -> -> -> , and the latter includes . In this situation, the functions are not yet declared, therefore we cannot provide the C++ aliases. */ #@INCLUDE_NEXT@ @NEXT_SYS_SOCKET_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_SYS_SOCKET_H #if @HAVE_SYS_SOCKET_H@ # define _GL_ALREADY_INCLUDING_SYS_SOCKET_H /* On many platforms, assumes prior inclusion of . */ # include /* On FreeBSD 6.4, defines some macros that assume that NULL is defined. */ # include /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_SYS_SOCKET_H@ # undef _GL_ALREADY_INCLUDING_SYS_SOCKET_H #endif #ifndef _@GUARD_PREFIX@_SYS_SOCKET_H #define _@GUARD_PREFIX@_SYS_SOCKET_H #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_SYS_SOCKET_INLINE # define _GL_SYS_SOCKET_INLINE _GL_INLINE #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #if !@HAVE_SA_FAMILY_T@ # if !GNULIB_defined_sa_family_t /* On OS/2 kLIBC, sa_family_t is unsigned char unless TCPV40HDRS is defined. */ # if !defined __KLIBC__ || defined TCPV40HDRS typedef unsigned short sa_family_t; # else typedef unsigned char sa_family_t; # endif # define GNULIB_defined_sa_family_t 1 # endif #endif #if @HAVE_STRUCT_SOCKADDR_STORAGE@ /* Make the 'struct sockaddr_storage' field 'ss_family' visible on AIX 7.1. */ # if !@HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ # ifndef ss_family # define ss_family __ss_family # endif # endif #else # include /* Code taken from glibc sysdeps/unix/sysv/linux/bits/socket.h on 2009-05-08, licensed under LGPLv2.1+, plus portability fixes. */ # define __ss_aligntype unsigned long int # define _SS_SIZE 256 # define _SS_PADSIZE \ (_SS_SIZE - ((sizeof (sa_family_t) >= alignof (__ss_aligntype) \ ? sizeof (sa_family_t) \ : alignof (__ss_aligntype)) \ + sizeof (__ss_aligntype))) # if !GNULIB_defined_struct_sockaddr_storage struct sockaddr_storage { sa_family_t ss_family; /* Address family, etc. */ __ss_aligntype __ss_align; /* Force desired alignment. */ char __ss_padding[_SS_PADSIZE]; }; # define GNULIB_defined_struct_sockaddr_storage 1 # endif #endif /* Get struct iovec. */ /* But avoid namespace pollution on glibc systems. */ #if ! defined __GLIBC__ # include #endif #if @HAVE_SYS_SOCKET_H@ /* A platform that has . */ /* For shutdown(). */ # if !defined SHUT_RD # define SHUT_RD 0 # endif # if !defined SHUT_WR # define SHUT_WR 1 # endif # if !defined SHUT_RDWR # define SHUT_RDWR 2 # endif # ifdef __VMS /* OpenVMS */ # ifndef CMSG_SPACE # define CMSG_SPACE(length) _CMSG_SPACE(length) # endif # ifndef CMSG_LEN # define CMSG_LEN(length) _CMSG_LEN(length) # endif # endif #else # ifdef __CYGWIN__ # error "Cygwin does have a sys/socket.h, doesn't it?!?" # endif /* A platform that lacks . Currently only MinGW is supported. See the gnulib manual regarding Windows sockets. MinGW has the header files winsock2.h and ws2tcpip.h that declare the sys/socket.h definitions we need. Note that you can influence which definitions you get by setting the WINVER symbol before including these two files. For example, getaddrinfo is only available if _WIN32_WINNT >= 0x0501 (that symbol is set indirectly through WINVER). You can set this by adding AC_DEFINE(WINVER, 0x0501) to configure.ac. Note that your code may not run on older Windows releases then. My Windows 2000 box was not able to run the code, for example. The situation is slightly confusing because suggests that getaddrinfo should be available on all Windows releases. */ # if @HAVE_WINSOCK2_H@ # include # endif # if @HAVE_WS2TCPIP_H@ # include # endif /* For shutdown(). */ # if !defined SHUT_RD && defined SD_RECEIVE # define SHUT_RD SD_RECEIVE # endif # if !defined SHUT_WR && defined SD_SEND # define SHUT_WR SD_SEND # endif # if !defined SHUT_RDWR && defined SD_BOTH # define SHUT_RDWR SD_BOTH # endif # if @HAVE_WINSOCK2_H@ /* Include headers needed by the emulation code. */ # include # include # if !GNULIB_defined_socklen_t typedef int socklen_t; # define GNULIB_defined_socklen_t 1 # endif # endif /* Rudimentary 'struct msghdr'; this works as long as you don't try to access msg_control or msg_controllen. */ struct msghdr { void *msg_name; socklen_t msg_namelen; struct iovec *msg_iov; int msg_iovlen; int msg_flags; }; #endif /* Fix some definitions from . */ #if @HAVE_WINSOCK2_H@ # if !GNULIB_defined_rpl_fd_isset /* Re-define FD_ISSET to avoid a WSA call while we are not using network sockets. */ _GL_SYS_SOCKET_INLINE int rpl_fd_isset (SOCKET fd, fd_set * set) { u_int i; if (set == NULL) return 0; for (i = 0; i < set->fd_count; i++) if (set->fd_array[i] == fd) return 1; return 0; } # define GNULIB_defined_rpl_fd_isset 1 # endif # undef FD_ISSET # define FD_ISSET(fd, set) rpl_fd_isset(fd, set) #endif /* Hide some function declarations from . */ #if @HAVE_WINSOCK2_H@ # if !defined _@GUARD_PREFIX@_UNISTD_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef close # define close close_used_without_including_unistd_h # else _GL_WARN_ON_USE (close, "close() used without including "); # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gethostname # define gethostname gethostname_used_without_including_unistd_h # else _GL_WARN_ON_USE (gethostname, "gethostname() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SELECT_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef select # define select select_used_without_including_sys_select_h # else _GL_WARN_ON_USE (select, "select() used without including "); # endif # endif #endif /* Wrap everything else to use libc file descriptors for sockets. */ #if @GNULIB_SOCKET@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef socket # define socket rpl_socket # endif _GL_FUNCDECL_RPL (socket, int, (int domain, int type, int protocol)); _GL_CXXALIAS_RPL (socket, int, (int domain, int type, int protocol)); # else _GL_CXXALIAS_SYS (socket, int, (int domain, int type, int protocol)); # endif _GL_CXXALIASWARN (socket); #elif @HAVE_WINSOCK2_H@ # undef socket # define socket socket_used_without_requesting_gnulib_module_socket #elif defined GNULIB_POSIXCHECK # undef socket # if HAVE_RAW_DECL_SOCKET _GL_WARN_ON_USE (socket, "socket is not always POSIX compliant - " "use gnulib module socket for portability"); # endif #endif #if @GNULIB_CONNECT@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef connect # define connect rpl_connect # endif _GL_FUNCDECL_RPL (connect, int, (int fd, const struct sockaddr *addr, socklen_t addrlen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (connect, int, (int fd, const struct sockaddr *addr, socklen_t addrlen)); # else /* Need to cast, because on NonStop Kernel, the third parameter is size_t addrlen. */ _GL_CXXALIAS_SYS_CAST (connect, int, (int fd, const struct sockaddr *addr, socklen_t addrlen)); # endif _GL_CXXALIASWARN (connect); #elif @HAVE_WINSOCK2_H@ # undef connect # define connect socket_used_without_requesting_gnulib_module_connect #elif defined GNULIB_POSIXCHECK # undef connect # if HAVE_RAW_DECL_CONNECT _GL_WARN_ON_USE (connect, "connect is not always POSIX compliant - " "use gnulib module connect for portability"); # endif #endif #if @GNULIB_ACCEPT@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef accept # define accept rpl_accept # endif _GL_FUNCDECL_RPL (accept, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); _GL_CXXALIAS_RPL (accept, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); # else /* Need to cast, because on Solaris 10 systems, the third parameter is void *addrlen. */ _GL_CXXALIAS_SYS_CAST (accept, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); # endif _GL_CXXALIASWARN (accept); #elif @HAVE_WINSOCK2_H@ # undef accept # define accept accept_used_without_requesting_gnulib_module_accept #elif defined GNULIB_POSIXCHECK # undef accept # if HAVE_RAW_DECL_ACCEPT _GL_WARN_ON_USE (accept, "accept is not always POSIX compliant - " "use gnulib module accept for portability"); # endif #endif #if @GNULIB_BIND@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef bind # define bind rpl_bind # endif _GL_FUNCDECL_RPL (bind, int, (int fd, const struct sockaddr *addr, socklen_t addrlen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (bind, int, (int fd, const struct sockaddr *addr, socklen_t addrlen)); # else /* Need to cast, because on NonStop Kernel, the third parameter is size_t addrlen. */ _GL_CXXALIAS_SYS_CAST (bind, int, (int fd, const struct sockaddr *addr, socklen_t addrlen)); # endif _GL_CXXALIASWARN (bind); #elif @HAVE_WINSOCK2_H@ # undef bind # define bind bind_used_without_requesting_gnulib_module_bind #elif defined GNULIB_POSIXCHECK # undef bind # if HAVE_RAW_DECL_BIND _GL_WARN_ON_USE (bind, "bind is not always POSIX compliant - " "use gnulib module bind for portability"); # endif #endif #if @GNULIB_GETPEERNAME@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getpeername # define getpeername rpl_getpeername # endif _GL_FUNCDECL_RPL (getpeername, int, (int fd, struct sockaddr *addr, socklen_t *addrlen) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (getpeername, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); # else /* Need to cast, because on Solaris 10 systems, the third parameter is void *addrlen. */ _GL_CXXALIAS_SYS_CAST (getpeername, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); # endif _GL_CXXALIASWARN (getpeername); #elif @HAVE_WINSOCK2_H@ # undef getpeername # define getpeername getpeername_used_without_requesting_gnulib_module_getpeername #elif defined GNULIB_POSIXCHECK # undef getpeername # if HAVE_RAW_DECL_GETPEERNAME _GL_WARN_ON_USE (getpeername, "getpeername is not always POSIX compliant - " "use gnulib module getpeername for portability"); # endif #endif #if @GNULIB_GETSOCKNAME@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getsockname # define getsockname rpl_getsockname # endif _GL_FUNCDECL_RPL (getsockname, int, (int fd, struct sockaddr *addr, socklen_t *addrlen) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (getsockname, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); # else /* Need to cast, because on Solaris 10 systems, the third parameter is void *addrlen. */ _GL_CXXALIAS_SYS_CAST (getsockname, int, (int fd, struct sockaddr *addr, socklen_t *addrlen)); # endif _GL_CXXALIASWARN (getsockname); #elif @HAVE_WINSOCK2_H@ # undef getsockname # define getsockname getsockname_used_without_requesting_gnulib_module_getsockname #elif defined GNULIB_POSIXCHECK # undef getsockname # if HAVE_RAW_DECL_GETSOCKNAME _GL_WARN_ON_USE (getsockname, "getsockname is not always POSIX compliant - " "use gnulib module getsockname for portability"); # endif #endif #if @GNULIB_GETSOCKOPT@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getsockopt # define getsockopt rpl_getsockopt # endif _GL_FUNCDECL_RPL (getsockopt, int, (int fd, int level, int optname, void *optval, socklen_t *optlen) _GL_ARG_NONNULL ((4, 5))); _GL_CXXALIAS_RPL (getsockopt, int, (int fd, int level, int optname, void *optval, socklen_t *optlen)); # else /* Need to cast, because on Solaris 10 systems, the fifth parameter is void *optlen. */ _GL_CXXALIAS_SYS_CAST (getsockopt, int, (int fd, int level, int optname, void *optval, socklen_t *optlen)); # endif _GL_CXXALIASWARN (getsockopt); #elif @HAVE_WINSOCK2_H@ # undef getsockopt # define getsockopt getsockopt_used_without_requesting_gnulib_module_getsockopt #elif defined GNULIB_POSIXCHECK # undef getsockopt # if HAVE_RAW_DECL_GETSOCKOPT _GL_WARN_ON_USE (getsockopt, "getsockopt is not always POSIX compliant - " "use gnulib module getsockopt for portability"); # endif #endif #if @GNULIB_LISTEN@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef listen # define listen rpl_listen # endif _GL_FUNCDECL_RPL (listen, int, (int fd, int backlog)); _GL_CXXALIAS_RPL (listen, int, (int fd, int backlog)); # else _GL_CXXALIAS_SYS (listen, int, (int fd, int backlog)); # endif _GL_CXXALIASWARN (listen); #elif @HAVE_WINSOCK2_H@ # undef listen # define listen listen_used_without_requesting_gnulib_module_listen #elif defined GNULIB_POSIXCHECK # undef listen # if HAVE_RAW_DECL_LISTEN _GL_WARN_ON_USE (listen, "listen is not always POSIX compliant - " "use gnulib module listen for portability"); # endif #endif #if @GNULIB_RECV@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef recv # define recv rpl_recv # endif _GL_FUNCDECL_RPL (recv, ssize_t, (int fd, void *buf, size_t len, int flags) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (recv, ssize_t, (int fd, void *buf, size_t len, int flags)); # else _GL_CXXALIAS_SYS (recv, ssize_t, (int fd, void *buf, size_t len, int flags)); # endif _GL_CXXALIASWARN (recv); #elif @HAVE_WINSOCK2_H@ # undef recv # define recv recv_used_without_requesting_gnulib_module_recv #elif defined GNULIB_POSIXCHECK # undef recv # if HAVE_RAW_DECL_RECV _GL_WARN_ON_USE (recv, "recv is not always POSIX compliant - " "use gnulib module recv for portability"); # endif #endif #if @GNULIB_SEND@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef send # define send rpl_send # endif _GL_FUNCDECL_RPL (send, ssize_t, (int fd, const void *buf, size_t len, int flags) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (send, ssize_t, (int fd, const void *buf, size_t len, int flags)); # else _GL_CXXALIAS_SYS (send, ssize_t, (int fd, const void *buf, size_t len, int flags)); # endif _GL_CXXALIASWARN (send); #elif @HAVE_WINSOCK2_H@ # undef send # define send send_used_without_requesting_gnulib_module_send #elif defined GNULIB_POSIXCHECK # undef send # if HAVE_RAW_DECL_SEND _GL_WARN_ON_USE (send, "send is not always POSIX compliant - " "use gnulib module send for portability"); # endif #endif #if @GNULIB_RECVFROM@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef recvfrom # define recvfrom rpl_recvfrom # endif _GL_FUNCDECL_RPL (recvfrom, ssize_t, (int fd, void *buf, size_t len, int flags, struct sockaddr *from, socklen_t *fromlen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (recvfrom, ssize_t, (int fd, void *buf, size_t len, int flags, struct sockaddr *from, socklen_t *fromlen)); # else /* Need to cast, because on Solaris 10 systems, the sixth parameter is void *fromlen. */ _GL_CXXALIAS_SYS_CAST (recvfrom, ssize_t, (int fd, void *buf, size_t len, int flags, struct sockaddr *from, socklen_t *fromlen)); # endif _GL_CXXALIASWARN (recvfrom); #elif @HAVE_WINSOCK2_H@ # undef recvfrom # define recvfrom recvfrom_used_without_requesting_gnulib_module_recvfrom #elif defined GNULIB_POSIXCHECK # undef recvfrom # if HAVE_RAW_DECL_RECVFROM _GL_WARN_ON_USE (recvfrom, "recvfrom is not always POSIX compliant - " "use gnulib module recvfrom for portability"); # endif #endif #if @GNULIB_SENDTO@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sendto # define sendto rpl_sendto # endif _GL_FUNCDECL_RPL (sendto, ssize_t, (int fd, const void *buf, size_t len, int flags, const struct sockaddr *to, socklen_t tolen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (sendto, ssize_t, (int fd, const void *buf, size_t len, int flags, const struct sockaddr *to, socklen_t tolen)); # else /* Need to cast, because on NonStop Kernel, the sixth parameter is size_t tolen. */ _GL_CXXALIAS_SYS_CAST (sendto, ssize_t, (int fd, const void *buf, size_t len, int flags, const struct sockaddr *to, socklen_t tolen)); # endif _GL_CXXALIASWARN (sendto); #elif @HAVE_WINSOCK2_H@ # undef sendto # define sendto sendto_used_without_requesting_gnulib_module_sendto #elif defined GNULIB_POSIXCHECK # undef sendto # if HAVE_RAW_DECL_SENDTO _GL_WARN_ON_USE (sendto, "sendto is not always POSIX compliant - " "use gnulib module sendto for portability"); # endif #endif #if @GNULIB_SETSOCKOPT@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setsockopt # define setsockopt rpl_setsockopt # endif _GL_FUNCDECL_RPL (setsockopt, int, (int fd, int level, int optname, const void * optval, socklen_t optlen) _GL_ARG_NONNULL ((4))); _GL_CXXALIAS_RPL (setsockopt, int, (int fd, int level, int optname, const void * optval, socklen_t optlen)); # else /* Need to cast, because on NonStop Kernel, the fifth parameter is size_t optlen. */ _GL_CXXALIAS_SYS_CAST (setsockopt, int, (int fd, int level, int optname, const void * optval, socklen_t optlen)); # endif _GL_CXXALIASWARN (setsockopt); #elif @HAVE_WINSOCK2_H@ # undef setsockopt # define setsockopt setsockopt_used_without_requesting_gnulib_module_setsockopt #elif defined GNULIB_POSIXCHECK # undef setsockopt # if HAVE_RAW_DECL_SETSOCKOPT _GL_WARN_ON_USE (setsockopt, "setsockopt is not always POSIX compliant - " "use gnulib module setsockopt for portability"); # endif #endif #if @GNULIB_SHUTDOWN@ # if @HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef shutdown # define shutdown rpl_shutdown # endif _GL_FUNCDECL_RPL (shutdown, int, (int fd, int how)); _GL_CXXALIAS_RPL (shutdown, int, (int fd, int how)); # else _GL_CXXALIAS_SYS (shutdown, int, (int fd, int how)); # endif _GL_CXXALIASWARN (shutdown); #elif @HAVE_WINSOCK2_H@ # undef shutdown # define shutdown shutdown_used_without_requesting_gnulib_module_shutdown #elif defined GNULIB_POSIXCHECK # undef shutdown # if HAVE_RAW_DECL_SHUTDOWN _GL_WARN_ON_USE (shutdown, "shutdown is not always POSIX compliant - " "use gnulib module shutdown for portability"); # endif #endif #if @GNULIB_ACCEPT4@ /* Accept a connection on a socket, with specific opening flags. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). See also the Linux man page at . */ # if @HAVE_ACCEPT4@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define accept4 rpl_accept4 # endif _GL_FUNCDECL_RPL (accept4, int, (int sockfd, struct sockaddr *addr, socklen_t *addrlen, int flags)); _GL_CXXALIAS_RPL (accept4, int, (int sockfd, struct sockaddr *addr, socklen_t *addrlen, int flags)); # else _GL_FUNCDECL_SYS (accept4, int, (int sockfd, struct sockaddr *addr, socklen_t *addrlen, int flags)); _GL_CXXALIAS_SYS (accept4, int, (int sockfd, struct sockaddr *addr, socklen_t *addrlen, int flags)); # endif _GL_CXXALIASWARN (accept4); #elif defined GNULIB_POSIXCHECK # undef accept4 # if HAVE_RAW_DECL_ACCEPT4 _GL_WARN_ON_USE (accept4, "accept4 is unportable - " "use gnulib module accept4 for portability"); # endif #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_SYS_SOCKET_H */ #endif /* _@GUARD_PREFIX@_SYS_SOCKET_H */ #endif gnuastro-0.5/bootstrapped/tests/sys_select.in.h0000644000175000017500000002756713217200023016753 00000000000000/* Substitute for . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ # if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ # endif @PRAGMA_COLUMNS@ /* On OSF/1 and Solaris 2.6, and both include . On Cygwin, includes . Simply delegate to the system's header in this case. */ #if (@HAVE_SYS_SELECT_H@ \ && !defined _GL_SYS_SELECT_H_REDIRECT_FROM_SYS_TYPES_H \ && ((defined __osf__ && defined _SYS_TYPES_H_ \ && defined _OSF_SOURCE) \ || (defined __sun && defined _SYS_TYPES_H \ && (! (defined _XOPEN_SOURCE || defined _POSIX_C_SOURCE) \ || defined __EXTENSIONS__)))) # define _GL_SYS_SELECT_H_REDIRECT_FROM_SYS_TYPES_H # @INCLUDE_NEXT@ @NEXT_SYS_SELECT_H@ #elif (@HAVE_SYS_SELECT_H@ \ && (defined _CYGWIN_SYS_TIME_H \ || (!defined _GL_SYS_SELECT_H_REDIRECT_FROM_SYS_TIME_H \ && ((defined __osf__ && defined _SYS_TIME_H_ \ && defined _OSF_SOURCE) \ || (defined __sun && defined _SYS_TIME_H \ && (! (defined _XOPEN_SOURCE \ || defined _POSIX_C_SOURCE) \ || defined __EXTENSIONS__)))))) # define _GL_SYS_SELECT_H_REDIRECT_FROM_SYS_TIME_H # @INCLUDE_NEXT@ @NEXT_SYS_SELECT_H@ /* On IRIX 6.5, includes , which includes , which includes . At this point we cannot include , because that includes , which gives a syntax error because has not been completely processed. Simply delegate to the system's header in this case. */ #elif @HAVE_SYS_SELECT_H@ && defined __sgi && (defined _SYS_BSD_TYPES_H && !defined _GL_SYS_SELECT_H_REDIRECT_FROM_SYS_BSD_TYPES_H) # define _GL_SYS_SELECT_H_REDIRECT_FROM_SYS_BSD_TYPES_H # @INCLUDE_NEXT@ @NEXT_SYS_SELECT_H@ /* On OpenBSD 5.0, includes , which includes . At this point we cannot include , because that includes gnulib's pthread.h override, which gives a syntax error because /usr/include/pthread.h has not been completely processed. Simply delegate to the system's header in this case. */ #elif @HAVE_SYS_SELECT_H@ && defined __OpenBSD__ && (defined _PTHREAD_H_ && !defined PTHREAD_MUTEX_INITIALIZER) # @INCLUDE_NEXT@ @NEXT_SYS_SELECT_H@ #else #ifndef _@GUARD_PREFIX@_SYS_SELECT_H /* On many platforms, assumes prior inclusion of . Also, mingw defines sigset_t there, instead of in where it belongs. */ #include #if @HAVE_SYS_SELECT_H@ /* On OSF/1 4.0, provides only a forward declaration of 'struct timeval', and no definition of this type. Also, Mac OS X, AIX, HP-UX, IRIX, Solaris, Interix declare select() in . But avoid namespace pollution on glibc systems and "unknown type name" problems on Cygwin. */ # if !(defined __GLIBC__ || defined __CYGWIN__) # include # endif /* On AIX 7 and Solaris 10, provides an FD_ZERO implementation that relies on memset(), but without including . But in any case avoid namespace pollution on glibc systems. */ # if (defined __OpenBSD__ || defined _AIX || defined __sun || defined __osf__ || defined __BEOS__) \ && ! defined __GLIBC__ # include # endif /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_SYS_SELECT_H@ #endif /* Get definition of 'sigset_t'. But avoid namespace pollution on glibc systems and "unknown type name" problems on Cygwin. Do this after the include_next (for the sake of OpenBSD 5.0) but before the split double-inclusion guard (for the sake of Solaris). */ #if !((defined __GLIBC__ || defined __CYGWIN__) && !defined __UCLIBC__) # include #endif #ifndef _@GUARD_PREFIX@_SYS_SELECT_H #define _@GUARD_PREFIX@_SYS_SELECT_H #if !@HAVE_SYS_SELECT_H@ /* A platform that lacks . */ /* Get the 'struct timeval' and 'fd_set' types and the FD_* macros on most platforms. */ # include /* On HP-UX 11, provides an FD_ZERO implementation that relies on memset(), but without including . */ # if defined __hpux # include # endif /* On native Windows platforms: Get the 'fd_set' type. Get the close() declaration before we override it. */ # if @HAVE_WINSOCK2_H@ # if !defined _GL_INCLUDING_WINSOCK2_H # define _GL_INCLUDING_WINSOCK2_H # include # undef _GL_INCLUDING_WINSOCK2_H # endif # include # endif #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Fix some definitions from . */ #if @HAVE_WINSOCK2_H@ # if !GNULIB_defined_rpl_fd_isset /* Re-define FD_ISSET to avoid a WSA call while we are not using network sockets. */ static int rpl_fd_isset (SOCKET fd, fd_set * set) { u_int i; if (set == NULL) return 0; for (i = 0; i < set->fd_count; i++) if (set->fd_array[i] == fd) return 1; return 0; } # define GNULIB_defined_rpl_fd_isset 1 # endif # undef FD_ISSET # define FD_ISSET(fd, set) rpl_fd_isset(fd, set) #endif /* Hide some function declarations from . */ #if @HAVE_WINSOCK2_H@ # if !defined _@GUARD_PREFIX@_UNISTD_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef close # define close close_used_without_including_unistd_h # else _GL_WARN_ON_USE (close, "close() used without including "); # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gethostname # define gethostname gethostname_used_without_including_unistd_h # else _GL_WARN_ON_USE (gethostname, "gethostname() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SOCKET_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef socket # define socket socket_used_without_including_sys_socket_h # undef connect # define connect connect_used_without_including_sys_socket_h # undef accept # define accept accept_used_without_including_sys_socket_h # undef bind # define bind bind_used_without_including_sys_socket_h # undef getpeername # define getpeername getpeername_used_without_including_sys_socket_h # undef getsockname # define getsockname getsockname_used_without_including_sys_socket_h # undef getsockopt # define getsockopt getsockopt_used_without_including_sys_socket_h # undef listen # define listen listen_used_without_including_sys_socket_h # undef recv # define recv recv_used_without_including_sys_socket_h # undef send # define send send_used_without_including_sys_socket_h # undef recvfrom # define recvfrom recvfrom_used_without_including_sys_socket_h # undef sendto # define sendto sendto_used_without_including_sys_socket_h # undef setsockopt # define setsockopt setsockopt_used_without_including_sys_socket_h # undef shutdown # define shutdown shutdown_used_without_including_sys_socket_h # else _GL_WARN_ON_USE (socket, "socket() used without including "); _GL_WARN_ON_USE (connect, "connect() used without including "); _GL_WARN_ON_USE (accept, "accept() used without including "); _GL_WARN_ON_USE (bind, "bind() used without including "); _GL_WARN_ON_USE (getpeername, "getpeername() used without including "); _GL_WARN_ON_USE (getsockname, "getsockname() used without including "); _GL_WARN_ON_USE (getsockopt, "getsockopt() used without including "); _GL_WARN_ON_USE (listen, "listen() used without including "); _GL_WARN_ON_USE (recv, "recv() used without including "); _GL_WARN_ON_USE (send, "send() used without including "); _GL_WARN_ON_USE (recvfrom, "recvfrom() used without including "); _GL_WARN_ON_USE (sendto, "sendto() used without including "); _GL_WARN_ON_USE (setsockopt, "setsockopt() used without including "); _GL_WARN_ON_USE (shutdown, "shutdown() used without including "); # endif # endif #endif #if @GNULIB_PSELECT@ # if @REPLACE_PSELECT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef pselect # define pselect rpl_pselect # endif _GL_FUNCDECL_RPL (pselect, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timespec const *restrict, const sigset_t *restrict)); _GL_CXXALIAS_RPL (pselect, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timespec const *restrict, const sigset_t *restrict)); # else # if !@HAVE_PSELECT@ _GL_FUNCDECL_SYS (pselect, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timespec const *restrict, const sigset_t *restrict)); # endif _GL_CXXALIAS_SYS (pselect, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timespec const *restrict, const sigset_t *restrict)); # endif _GL_CXXALIASWARN (pselect); #elif defined GNULIB_POSIXCHECK # undef pselect # if HAVE_RAW_DECL_PSELECT _GL_WARN_ON_USE (pselect, "pselect is not portable - " "use gnulib module pselect for portability"); # endif #endif #if @GNULIB_SELECT@ # if @REPLACE_SELECT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef select # define select rpl_select # endif _GL_FUNCDECL_RPL (select, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timeval *restrict)); _GL_CXXALIAS_RPL (select, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timeval *restrict)); # else _GL_CXXALIAS_SYS (select, int, (int, fd_set *restrict, fd_set *restrict, fd_set *restrict, struct timeval *restrict)); # endif _GL_CXXALIASWARN (select); #elif @HAVE_WINSOCK2_H@ # undef select # define select select_used_without_requesting_gnulib_module_select #elif defined GNULIB_POSIXCHECK # undef select # if HAVE_RAW_DECL_SELECT _GL_WARN_ON_USE (select, "select is not always POSIX compliant - " "use gnulib module select for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_SYS_SELECT_H */ #endif /* _@GUARD_PREFIX@_SYS_SELECT_H */ #endif /* OSF/1 */ gnuastro-0.5/bootstrapped/tests/sys_ioctl.in.h0000644000175000017500000000501313217200023016564 00000000000000/* Substitute for and wrapper around . Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_SYS_IOCTL_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_SYS_IOCTL_H@ # @INCLUDE_NEXT@ @NEXT_SYS_IOCTL_H@ #endif #ifndef _@GUARD_PREFIX@_SYS_IOCTL_H #define _@GUARD_PREFIX@_SYS_IOCTL_H /* AIX 5.1 and Solaris 10 declare ioctl() in and in , but not in . Haiku declares ioctl() in , but not in . But avoid namespace pollution on glibc systems. */ #ifndef __GLIBC__ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Declare overridden functions. */ #if @GNULIB_IOCTL@ # if @REPLACE_IOCTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ioctl # define ioctl rpl_ioctl # endif _GL_FUNCDECL_RPL (ioctl, int, (int fd, int request, ... /* {void *,char *} arg */)); _GL_CXXALIAS_RPL (ioctl, int, (int fd, int request, ... /* {void *,char *} arg */)); # else # if @SYS_IOCTL_H_HAVE_WINSOCK2_H@ || 1 _GL_FUNCDECL_SYS (ioctl, int, (int fd, int request, ... /* {void *,char *} arg */)); # endif _GL_CXXALIAS_SYS (ioctl, int, (int fd, int request, ... /* {void *,char *} arg */)); # endif _GL_CXXALIASWARN (ioctl); #elif @SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ # undef ioctl # define ioctl ioctl_used_without_requesting_gnulib_module_ioctl #elif defined GNULIB_POSIXCHECK # undef ioctl # if HAVE_RAW_DECL_IOCTL _GL_WARN_ON_USE (ioctl, "ioctl does not portably work on sockets - " "use gnulib module ioctl for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_SYS_IOCTL_H */ #endif /* _@GUARD_PREFIX@_SYS_IOCTL_H */ gnuastro-0.5/bootstrapped/tests/test-symlink.h0000644000175000017500000000607113217200024016620 00000000000000/* Tests of symlink. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ /* This file is designed to test both symlink(a,b) and symlinkat(a,AT_FDCWD,b). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static int test_symlink (int (*func) (char const *, char const *), bool print) { if (func ("nowhere", BASE "link1")) { if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } /* Some systems allow the creation of 0-length symlinks as a synonym for "."; but most reject it. */ { int status; errno = 0; status = func ("", BASE "link2"); if (status == -1) ASSERT (errno == ENOENT || errno == EINVAL); else { ASSERT (status == 0); ASSERT (unlink (BASE "link2") == 0); } } /* Sanity checks of failures. */ errno = 0; ASSERT (func ("nowhere", "") == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nowhere", ".") == -1); ASSERT (errno == EEXIST || errno == EINVAL); errno = 0; ASSERT (func ("somewhere", BASE "link1") == -1); ASSERT (errno == EEXIST); errno = 0; ASSERT (func ("nowhere", BASE "link2/") == -1); ASSERT (errno == ENOTDIR || errno == ENOENT); ASSERT (mkdir (BASE "dir", 0700) == 0); errno = 0; ASSERT (func ("nowhere", BASE "dir") == -1); ASSERT (errno == EEXIST); errno = 0; ASSERT (func ("nowhere", BASE "dir/") == -1); ASSERT (errno == EEXIST || errno == EINVAL); ASSERT (close (creat (BASE "file", 0600)) == 0); errno = 0; ASSERT (func ("nowhere", BASE "file") == -1); ASSERT (errno == EEXIST); errno = 0; ASSERT (func ("nowhere", BASE "file/") == -1); ASSERT (errno == EEXIST || errno == ENOTDIR || errno == ENOENT); /* Trailing slash must always be rejected. */ ASSERT (unlink (BASE "link1") == 0); ASSERT (func (BASE "link2", BASE "link1") == 0); errno = 0; ASSERT (func (BASE "nowhere", BASE "link1/") == -1); ASSERT (errno == EEXIST || errno == ENOTDIR || errno == ENOENT); errno = 0; ASSERT (unlink (BASE "link2") == -1); ASSERT (errno == ENOENT); /* Cleanup. */ ASSERT (rmdir (BASE "dir") == 0); ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link1") == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-sys_wait.h0000644000175000017500000000361613217200024016776 00000000000000/* Test of macros shared between and . Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2010. */ static int test_sys_wait_macros (void) { /* Check subset of macros that must be visible here. Note that some of these macros are only portable when operating on an lvalue. */ int i; for (i = 0; i < 0x8000; i = (i ? i << 1 : 1)) { /* POSIX requires that for all valid process statuses, that exactly one of these three macros is true. But not all possible 16-bit values map to valid process status. Traditionally, 8 of the bits are for WIFEXITED, 7 of the bits to tell between WIFSIGNALED and WIFSTOPPED, and either 0x80 or 0x8000 to flag that core was also dumped. Since we don't know which byte is WIFEXITED, we skip the both possible bits that can signal core dump. */ if (i == 0x80) continue; if (!!WIFSIGNALED (i) + !!WIFEXITED (i) + !!WIFSTOPPED (i) != 1) return 1; } i = WEXITSTATUS (i) + WSTOPSIG (i) + WTERMSIG (i); switch (i) { #if 0 /* Gnulib doesn't guarantee these, yet. */ case WNOHANG: case WUNTRACED: #endif break; } return 0; } gnuastro-0.5/bootstrapped/tests/nap.h0000644000175000017500000001025113217200023014725 00000000000000/* Assist in file system timestamp tests. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #ifndef GLTEST_NAP_H # define GLTEST_NAP_H # include # include # include /* Name of the witness file. */ #define TEMPFILE BASE "nap.tmp" /* File descriptor used for the witness file. */ static int nap_fd = -1; /* Return A - B, in ns. Return 0 if the true result would be negative. Return INT_MAX if the true result would be greater than INT_MAX. */ static int diff_timespec (struct timespec a, struct timespec b) { time_t as = a.tv_sec; time_t bs = b.tv_sec; int ans = a.tv_nsec; int bns = b.tv_nsec; int sdiff; ASSERT (0 <= ans && ans < 2000000000); ASSERT (0 <= bns && bns < 2000000000); if (! (bs < as || (bs == as && bns < ans))) return 0; if (INT_SUBTRACT_WRAPV (as, bs, &sdiff) || INT_MULTIPLY_WRAPV (sdiff, 1000000000, &sdiff) || INT_ADD_WRAPV (sdiff, ans - bns, &sdiff)) return INT_MAX; return sdiff; } /* If DO_WRITE, bump the modification time of the file designated by NAP_FD. Then fetch the new STAT information of NAP_FD. */ static void nap_get_stat (struct stat *st, int do_write) { if (do_write) { ASSERT (write (nap_fd, "\n", 1) == 1); #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the modification times are not changed until NAP_FD is closed. See https://msdn.microsoft.com/en-us/library/windows/desktop/aa365747(v=vs.85).aspx */ close (nap_fd); nap_fd = open (TEMPFILE, O_RDWR, 0600); ASSERT (nap_fd != -1); lseek (nap_fd, 0, SEEK_END); #endif } ASSERT (fstat (nap_fd, st) == 0); } /* Given a file whose descriptor is FD, see whether delaying by DELAY nanoseconds causes a change in a file's mtime. OLD_ST is the file's status, recently gotten. */ static bool nap_works (int delay, struct stat old_st) { struct stat st; struct timespec delay_spec; delay_spec.tv_sec = delay / 1000000000; delay_spec.tv_nsec = delay % 1000000000; ASSERT (nanosleep (&delay_spec, 0) == 0); nap_get_stat (&st, 1); if (diff_timespec (get_stat_mtime (&st), get_stat_mtime (&old_st))) return true; return false; } static void clear_temp_file (void) { if (0 <= nap_fd) { ASSERT (close (nap_fd) != -1); ASSERT (unlink (TEMPFILE) != -1); } } /* Sleep long enough to notice a timestamp difference on the file system in the current directory. Use an adaptive approach, trying to find the smallest delay which works on the current file system to make the timestamp difference appear. Assert a maximum delay of ~2 seconds, more precisely sum(2^n) from 0 to 30 = 2^31 - 1 = 2.1s. Assumes that BASE is defined, and requires that the test module depends on nanosleep. */ static void nap (void) { struct stat old_st; static int delay = 1; if (-1 == nap_fd) { atexit (clear_temp_file); ASSERT ((nap_fd = creat (TEMPFILE, 0600)) != -1); nap_get_stat (&old_st, 0); } else { ASSERT (0 <= nap_fd); nap_get_stat (&old_st, 1); } if (1 < delay) delay = delay / 2; /* Try half of the previous delay. */ ASSERT (0 < delay); for (;;) { if (nap_works (delay, old_st)) return; if (delay <= (2147483647 - 1) / 2) { delay = delay * 2 + 1; continue; } else break; } /* Bummer: even the highest nap delay didn't work. */ ASSERT (0); } #endif /* GLTEST_NAP_H */ gnuastro-0.5/bootstrapped/tests/stat-time.h0000644000175000017500000001717313217200023016070 00000000000000/* stat-related time functions. Copyright (C) 2005, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ #ifndef STAT_TIME_H #define STAT_TIME_H 1 #include "intprops.h" #include #include #include #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_STAT_TIME_INLINE # define _GL_STAT_TIME_INLINE _GL_INLINE #endif #ifdef __cplusplus extern "C" { #endif /* STAT_TIMESPEC (ST, ST_XTIM) is the ST_XTIM member for *ST of type struct timespec, if available. If not, then STAT_TIMESPEC_NS (ST, ST_XTIM) is the nanosecond component of the ST_XTIM member for *ST, if available. ST_XTIM can be st_atim, st_ctim, st_mtim, or st_birthtim for access, status change, data modification, or birth (creation) time respectively. These macros are private to stat-time.h. */ #if _GL_WINDOWS_STAT_TIMESPEC || defined HAVE_STRUCT_STAT_ST_ATIM_TV_NSEC # if _GL_WINDOWS_STAT_TIMESPEC || defined TYPEOF_STRUCT_STAT_ST_ATIM_IS_STRUCT_TIMESPEC # define STAT_TIMESPEC(st, st_xtim) ((st)->st_xtim) # else # define STAT_TIMESPEC_NS(st, st_xtim) ((st)->st_xtim.tv_nsec) # endif #elif defined HAVE_STRUCT_STAT_ST_ATIMESPEC_TV_NSEC # define STAT_TIMESPEC(st, st_xtim) ((st)->st_xtim##espec) #elif defined HAVE_STRUCT_STAT_ST_ATIMENSEC # define STAT_TIMESPEC_NS(st, st_xtim) ((st)->st_xtim##ensec) #elif defined HAVE_STRUCT_STAT_ST_ATIM_ST__TIM_TV_NSEC # define STAT_TIMESPEC_NS(st, st_xtim) ((st)->st_xtim.st__tim.tv_nsec) #endif /* Return the nanosecond component of *ST's access time. */ _GL_STAT_TIME_INLINE long int _GL_ATTRIBUTE_PURE get_stat_atime_ns (struct stat const *st) { # if defined STAT_TIMESPEC return STAT_TIMESPEC (st, st_atim).tv_nsec; # elif defined STAT_TIMESPEC_NS return STAT_TIMESPEC_NS (st, st_atim); # else return 0; # endif } /* Return the nanosecond component of *ST's status change time. */ _GL_STAT_TIME_INLINE long int _GL_ATTRIBUTE_PURE get_stat_ctime_ns (struct stat const *st) { # if defined STAT_TIMESPEC return STAT_TIMESPEC (st, st_ctim).tv_nsec; # elif defined STAT_TIMESPEC_NS return STAT_TIMESPEC_NS (st, st_ctim); # else return 0; # endif } /* Return the nanosecond component of *ST's data modification time. */ _GL_STAT_TIME_INLINE long int _GL_ATTRIBUTE_PURE get_stat_mtime_ns (struct stat const *st) { # if defined STAT_TIMESPEC return STAT_TIMESPEC (st, st_mtim).tv_nsec; # elif defined STAT_TIMESPEC_NS return STAT_TIMESPEC_NS (st, st_mtim); # else return 0; # endif } /* Return the nanosecond component of *ST's birth time. */ _GL_STAT_TIME_INLINE long int _GL_ATTRIBUTE_PURE get_stat_birthtime_ns (struct stat const *st) { # if defined HAVE_STRUCT_STAT_ST_BIRTHTIMESPEC_TV_NSEC return STAT_TIMESPEC (st, st_birthtim).tv_nsec; # elif defined HAVE_STRUCT_STAT_ST_BIRTHTIMENSEC return STAT_TIMESPEC_NS (st, st_birthtim); # else /* Avoid a "parameter unused" warning. */ (void) st; return 0; # endif } /* Return *ST's access time. */ _GL_STAT_TIME_INLINE struct timespec _GL_ATTRIBUTE_PURE get_stat_atime (struct stat const *st) { #ifdef STAT_TIMESPEC return STAT_TIMESPEC (st, st_atim); #else struct timespec t; t.tv_sec = st->st_atime; t.tv_nsec = get_stat_atime_ns (st); return t; #endif } /* Return *ST's status change time. */ _GL_STAT_TIME_INLINE struct timespec _GL_ATTRIBUTE_PURE get_stat_ctime (struct stat const *st) { #ifdef STAT_TIMESPEC return STAT_TIMESPEC (st, st_ctim); #else struct timespec t; t.tv_sec = st->st_ctime; t.tv_nsec = get_stat_ctime_ns (st); return t; #endif } /* Return *ST's data modification time. */ _GL_STAT_TIME_INLINE struct timespec _GL_ATTRIBUTE_PURE get_stat_mtime (struct stat const *st) { #ifdef STAT_TIMESPEC return STAT_TIMESPEC (st, st_mtim); #else struct timespec t; t.tv_sec = st->st_mtime; t.tv_nsec = get_stat_mtime_ns (st); return t; #endif } /* Return *ST's birth time, if available; otherwise return a value with tv_sec and tv_nsec both equal to -1. */ _GL_STAT_TIME_INLINE struct timespec _GL_ATTRIBUTE_PURE get_stat_birthtime (struct stat const *st) { struct timespec t; #if (defined HAVE_STRUCT_STAT_ST_BIRTHTIMESPEC_TV_NSEC \ || defined HAVE_STRUCT_STAT_ST_BIRTHTIM_TV_NSEC) t = STAT_TIMESPEC (st, st_birthtim); #elif defined HAVE_STRUCT_STAT_ST_BIRTHTIMENSEC t.tv_sec = st->st_birthtime; t.tv_nsec = st->st_birthtimensec; #elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Native Windows platforms (but not Cygwin) put the "file creation time" in st_ctime (!). See . */ # if _GL_WINDOWS_STAT_TIMESPEC t = st->st_ctim; # else t.tv_sec = st->st_ctime; t.tv_nsec = 0; # endif #else /* Birth time is not supported. */ t.tv_sec = -1; t.tv_nsec = -1; /* Avoid a "parameter unused" warning. */ (void) st; #endif #if (defined HAVE_STRUCT_STAT_ST_BIRTHTIMESPEC_TV_NSEC \ || defined HAVE_STRUCT_STAT_ST_BIRTHTIM_TV_NSEC \ || defined HAVE_STRUCT_STAT_ST_BIRTHTIMENSEC) /* FreeBSD and NetBSD sometimes signal the absence of knowledge by using zero. Attempt to work around this problem. Alas, this can report failure even for valid timestamps. Also, NetBSD sometimes returns junk in the birth time fields; work around this bug if it is detected. */ if (! (t.tv_sec && 0 <= t.tv_nsec && t.tv_nsec < 1000000000)) { t.tv_sec = -1; t.tv_nsec = -1; } #endif return t; } /* If a stat-like function returned RESULT, normalize the timestamps in *ST, in case this platform suffers from the Solaris 11 bug where tv_nsec might be negative. Return the adjusted RESULT, setting errno to EOVERFLOW if normalization overflowed. This function is intended to be private to this .h file. */ _GL_STAT_TIME_INLINE int stat_time_normalize (int result, struct stat *st) { #if defined __sun && defined STAT_TIMESPEC if (result == 0) { long int timespec_resolution = 1000000000; short int const ts_off[] = { offsetof (struct stat, st_atim), offsetof (struct stat, st_mtim), offsetof (struct stat, st_ctim) }; int i; for (i = 0; i < sizeof ts_off / sizeof *ts_off; i++) { struct timespec *ts = (struct timespec *) ((char *) st + ts_off[i]); long int q = ts->tv_nsec / timespec_resolution; long int r = ts->tv_nsec % timespec_resolution; if (r < 0) { r += timespec_resolution; q--; } ts->tv_nsec = r; /* Overflow is possible, as Solaris 11 stat can yield tv_sec == TYPE_MINIMUM (time_t) && tv_nsec == -1000000000. INT_ADD_WRAPV is OK, since time_t is signed on Solaris. */ if (INT_ADD_WRAPV (q, ts->tv_sec, &ts->tv_sec)) { errno = EOVERFLOW; return -1; } } } #endif return result; } #ifdef __cplusplus } #endif _GL_INLINE_HEADER_END #endif gnuastro-0.5/bootstrapped/tests/test-stat.h0000644000175000017500000000604313217200024016104 00000000000000/* Tests of stat. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ /* This file is designed to test both stat(n,buf) and fstatat(AT_FDCWD,n,buf,0). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static int test_stat_func (int (*func) (char const *, struct stat *), bool print) { struct stat st1; struct stat st2; char *cwd = getcwd (NULL, 0); ASSERT (cwd); ASSERT (func (".", &st1) == 0); ASSERT (func ("./", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (func (cwd, &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (func ("/", &st1) == 0); ASSERT (func ("///", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); errno = 0; ASSERT (func ("", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch/", &st1) == -1); ASSERT (errno == ENOENT); ASSERT (close (creat (BASE "file", 0600)) == 0); ASSERT (func (BASE "file", &st1) == 0); errno = 0; ASSERT (func (BASE "file/", &st1) == -1); ASSERT (errno == ENOTDIR); /* Now for some symlink tests, where supported. We set up: link1 -> directory link2 -> file link3 -> dangling link4 -> loop then test behavior with trailing slash. */ if (symlink (".", BASE "link1") != 0) { ASSERT (unlink (BASE "file") == 0); if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } ASSERT (symlink (BASE "file", BASE "link2") == 0); ASSERT (symlink (BASE "nosuch", BASE "link3") == 0); ASSERT (symlink (BASE "link4", BASE "link4") == 0); ASSERT (func (BASE "link1/", &st1) == 0); ASSERT (S_ISDIR (st1.st_mode)); errno = 0; ASSERT (func (BASE "link2/", &st1) == -1); ASSERT (errno == ENOTDIR); errno = 0; ASSERT (func (BASE "link3/", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func (BASE "link4/", &st1) == -1); ASSERT (errno == ELOOP); /* Cleanup. */ ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link1") == 0); ASSERT (unlink (BASE "link2") == 0); ASSERT (unlink (BASE "link3") == 0); ASSERT (unlink (BASE "link4") == 0); free (cwd); return 0; } gnuastro-0.5/bootstrapped/tests/warn-on-use.h0000644000175000017500000001201013217200024016316 00000000000000/* A C macro for emitting warnings if a function is used. Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* _GL_WARN_ON_USE (function, "literal string") issues a declaration for FUNCTION which will then trigger a compiler warning containing the text of "literal string" anywhere that function is called, if supported by the compiler. If the compiler does not support this feature, the macro expands to an unused extern declaration. This macro is useful for marking a function as a potential portability trap, with the intent that "literal string" include instructions on the replacement function that should be used instead. However, one of the reasons that a function is a portability trap is if it has the wrong signature. Declaring FUNCTION with a different signature in C is a compilation error, so this macro must use the same type as any existing declaration so that programs that avoid the problematic FUNCTION do not fail to compile merely because they included a header that poisoned the function. But this implies that _GL_WARN_ON_USE is only safe to use if FUNCTION is known to already have a declaration. Use of this macro implies that there must not be any other macro hiding the declaration of FUNCTION; but undefining FUNCTION first is part of the poisoning process anyway (although for symbols that are provided only via a macro, the result is a compilation error rather than a warning containing "literal string"). Also note that in C++, it is only safe to use if FUNCTION has no overloads. For an example, it is possible to poison 'getline' by: - adding a call to gl_WARN_ON_USE_PREPARE([[#include ]], [getline]) in configure.ac, which potentially defines HAVE_RAW_DECL_GETLINE - adding this code to a header that wraps the system : #undef getline #if HAVE_RAW_DECL_GETLINE _GL_WARN_ON_USE (getline, "getline is required by POSIX 2008, but" "not universally present; use the gnulib module getline"); #endif It is not possible to directly poison global variables. But it is possible to write a wrapper accessor function, and poison that (less common usage, like &environ, will cause a compilation error rather than issue the nice warning, but the end result of informing the developer about their portability problem is still achieved): #if HAVE_RAW_DECL_ENVIRON static char ***rpl_environ (void) { return &environ; } _GL_WARN_ON_USE (rpl_environ, "environ is not always properly declared"); # undef environ # define environ (*rpl_environ ()) #endif */ #ifndef _GL_WARN_ON_USE # if 4 < __GNUC__ || (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) /* A compiler attribute is available in gcc versions 4.3.0 and later. */ # define _GL_WARN_ON_USE(function, message) \ extern __typeof__ (function) function __attribute__ ((__warning__ (message))) # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING /* Verify the existence of the function. */ # define _GL_WARN_ON_USE(function, message) \ extern __typeof__ (function) function # else /* Unsupported. */ # define _GL_WARN_ON_USE(function, message) \ _GL_WARN_EXTERN_C int _gl_warn_on_use # endif #endif /* _GL_WARN_ON_USE_CXX (function, rettype, parameters_and_attributes, "string") is like _GL_WARN_ON_USE (function, "string"), except that the function is declared with the given prototype, consisting of return type, parameters, and attributes. This variant is useful for overloaded functions in C++. _GL_WARN_ON_USE does not work in this case. */ #ifndef _GL_WARN_ON_USE_CXX # if 4 < __GNUC__ || (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ extern rettype function parameters_and_attributes \ __attribute__ ((__warning__ (msg))) # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING /* Verify the existence of the function. */ # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ extern rettype function parameters_and_attributes # else /* Unsupported. */ # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ _GL_WARN_EXTERN_C int _gl_warn_on_use # endif #endif /* _GL_WARN_EXTERN_C declaration; performs the declaration with C linkage. */ #ifndef _GL_WARN_EXTERN_C # if defined __cplusplus # define _GL_WARN_EXTERN_C extern "C" # else # define _GL_WARN_EXTERN_C extern # endif #endif gnuastro-0.5/bootstrapped/tests/c++defs.h0000644000175000017500000003413013217200022015362 00000000000000/* C++ compatible function declaration macros. Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_CXXDEFS_H #define _GL_CXXDEFS_H /* Begin/end the GNULIB_NAMESPACE namespace. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_BEGIN_NAMESPACE namespace GNULIB_NAMESPACE { # define _GL_END_NAMESPACE } #else # define _GL_BEGIN_NAMESPACE # define _GL_END_NAMESPACE #endif /* The three most frequent use cases of these macros are: * For providing a substitute for a function that is missing on some platforms, but is declared and works fine on the platforms on which it exists: #if @GNULIB_FOO@ # if !@HAVE_FOO@ _GL_FUNCDECL_SYS (foo, ...); # endif _GL_CXXALIAS_SYS (foo, ...); _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif * For providing a replacement for a function that exists on all platforms, but is broken/insufficient and needs to be replaced on some platforms: #if @GNULIB_FOO@ # if @REPLACE_FOO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef foo # define foo rpl_foo # endif _GL_FUNCDECL_RPL (foo, ...); _GL_CXXALIAS_RPL (foo, ...); # else _GL_CXXALIAS_SYS (foo, ...); # endif _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif * For providing a replacement for a function that exists on some platforms but is broken/insufficient and needs to be replaced on some of them and is additionally either missing or undeclared on some other platforms: #if @GNULIB_FOO@ # if @REPLACE_FOO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef foo # define foo rpl_foo # endif _GL_FUNCDECL_RPL (foo, ...); _GL_CXXALIAS_RPL (foo, ...); # else # if !@HAVE_FOO@ or if !@HAVE_DECL_FOO@ _GL_FUNCDECL_SYS (foo, ...); # endif _GL_CXXALIAS_SYS (foo, ...); # endif _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif */ /* _GL_EXTERN_C declaration; performs the declaration with C linkage. */ #if defined __cplusplus # define _GL_EXTERN_C extern "C" #else # define _GL_EXTERN_C extern #endif /* _GL_FUNCDECL_RPL (func, rettype, parameters_and_attributes); declares a replacement function, named rpl_func, with the given prototype, consisting of return type, parameters, and attributes. Example: _GL_FUNCDECL_RPL (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); */ #define _GL_FUNCDECL_RPL(func,rettype,parameters_and_attributes) \ _GL_FUNCDECL_RPL_1 (rpl_##func, rettype, parameters_and_attributes) #define _GL_FUNCDECL_RPL_1(rpl_func,rettype,parameters_and_attributes) \ _GL_EXTERN_C rettype rpl_func parameters_and_attributes /* _GL_FUNCDECL_SYS (func, rettype, parameters_and_attributes); declares the system function, named func, with the given prototype, consisting of return type, parameters, and attributes. Example: _GL_FUNCDECL_SYS (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); */ #define _GL_FUNCDECL_SYS(func,rettype,parameters_and_attributes) \ _GL_EXTERN_C rettype func parameters_and_attributes /* _GL_CXXALIAS_RPL (func, rettype, parameters); declares a C++ alias called GNULIB_NAMESPACE::func that redirects to rpl_func, if GNULIB_NAMESPACE is defined. Example: _GL_CXXALIAS_RPL (open, int, (const char *filename, int flags, ...)); Wrapping rpl_func in an object with an inline conversion operator avoids a reference to rpl_func unless GNULIB_NAMESPACE::func is actually used in the program. */ #define _GL_CXXALIAS_RPL(func,rettype,parameters) \ _GL_CXXALIAS_RPL_1 (func, rpl_##func, rettype, parameters) #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_RPL_1(func,rpl_func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return ::rpl_func; \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_RPL_1(func,rpl_func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_RPL_CAST_1 (func, rpl_func, rettype, parameters); is like _GL_CXXALIAS_RPL_1 (func, rpl_func, rettype, parameters); except that the C function rpl_func may have a slightly different declaration. A cast is used to silence the "invalid conversion" error that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_RPL_CAST_1(func,rpl_func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return reinterpret_cast(::rpl_func); \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_RPL_CAST_1(func,rpl_func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS (func, rettype, parameters); declares a C++ alias called GNULIB_NAMESPACE::func that redirects to the system provided function func, if GNULIB_NAMESPACE is defined. Example: _GL_CXXALIAS_SYS (open, int, (const char *filename, int flags, ...)); Wrapping func in an object with an inline conversion operator avoids a reference to func unless GNULIB_NAMESPACE::func is actually used in the program. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_SYS(func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return ::func; \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS(func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS_CAST (func, rettype, parameters); is like _GL_CXXALIAS_SYS (func, rettype, parameters); except that the C function func may have a slightly different declaration. A cast is used to silence the "invalid conversion" error that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_SYS_CAST(func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return reinterpret_cast(::func); \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS_CAST(func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS_CAST2 (func, rettype, parameters, rettype2, parameters2); is like _GL_CXXALIAS_SYS (func, rettype, parameters); except that the C function is picked among a set of overloaded functions, namely the one with rettype2 and parameters2. Two consecutive casts are used to silence the "cannot find a match" and "invalid conversion" errors that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE /* The outer cast must be a reinterpret_cast. The inner cast: When the function is defined as a set of overloaded functions, it works as a static_cast<>, choosing the designated variant. When the function is defined as a single variant, it works as a reinterpret_cast<>. The parenthesized cast syntax works both ways. */ # define _GL_CXXALIAS_SYS_CAST2(func,rettype,parameters,rettype2,parameters2) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return reinterpret_cast((rettype2 (*) parameters2)(::func)); \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS_CAST2(func,rettype,parameters,rettype2,parameters2) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIASWARN (func); causes a warning to be emitted when ::func is used but not when GNULIB_NAMESPACE::func is used. func must be defined without overloaded variants. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIASWARN(func) \ _GL_CXXALIASWARN_1 (func, GNULIB_NAMESPACE) # define _GL_CXXALIASWARN_1(func,namespace) \ _GL_CXXALIASWARN_2 (func, namespace) /* To work around GCC bug , we enable the warning only when not optimizing. */ # if !__OPTIMIZE__ # define _GL_CXXALIASWARN_2(func,namespace) \ _GL_WARN_ON_USE (func, \ "The symbol ::" #func " refers to the system function. " \ "Use " #namespace "::" #func " instead.") # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING # define _GL_CXXALIASWARN_2(func,namespace) \ extern __typeof__ (func) func # else # define _GL_CXXALIASWARN_2(func,namespace) \ _GL_EXTERN_C int _gl_cxxalias_dummy # endif #else # define _GL_CXXALIASWARN(func) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIASWARN1 (func, rettype, parameters_and_attributes); causes a warning to be emitted when the given overloaded variant of ::func is used but not when GNULIB_NAMESPACE::func is used. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIASWARN1(func,rettype,parameters_and_attributes) \ _GL_CXXALIASWARN1_1 (func, rettype, parameters_and_attributes, \ GNULIB_NAMESPACE) # define _GL_CXXALIASWARN1_1(func,rettype,parameters_and_attributes,namespace) \ _GL_CXXALIASWARN1_2 (func, rettype, parameters_and_attributes, namespace) /* To work around GCC bug , we enable the warning only when not optimizing. */ # if !__OPTIMIZE__ # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ _GL_WARN_ON_USE_CXX (func, rettype, parameters_and_attributes, \ "The symbol ::" #func " refers to the system function. " \ "Use " #namespace "::" #func " instead.") # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ extern __typeof__ (func) func # else # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ _GL_EXTERN_C int _gl_cxxalias_dummy # endif #else # define _GL_CXXALIASWARN1(func,rettype,parameters_and_attributes) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif #endif /* _GL_CXXDEFS_H */ gnuastro-0.5/bootstrapped/tests/arg-nonnull.h0000644000175000017500000000230113217200022016377 00000000000000/* A C macro for declaring that specific arguments must not be NULL. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* _GL_ARG_NONNULL((n,...,m)) tells the compiler and static analyzer tools that the values passed as arguments n, ..., m must be non-NULL pointers. n = 1 stands for the first argument, n = 2 for the second argument etc. */ #ifndef _GL_ARG_NONNULL # if (__GNUC__ == 3 && __GNUC_MINOR__ >= 3) || __GNUC__ > 3 # define _GL_ARG_NONNULL(params) __attribute__ ((__nonnull__ params)) # else # define _GL_ARG_NONNULL(params) # endif #endif gnuastro-0.5/bootstrapped/tests/_Noreturn.h0000644000175000017500000000046213217200022016124 00000000000000#if !defined _Noreturn && __STDC_VERSION__ < 201112 # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif gnuastro-0.5/bootstrapped/tests/signal.in.h0000644000175000017500000003461213217200023016040 00000000000000/* A GNU-like . Copyright (C) 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_sig_atomic_t || defined __need_sigset_t || defined _GL_ALREADY_INCLUDING_SIGNAL_H || (defined _SIGNAL_H && !defined __SIZEOF_PTHREAD_MUTEX_T) /* Special invocation convention: - Inside glibc header files. - On glibc systems we have a sequence of nested includes -> -> . In this situation, the functions are not yet declared, therefore we cannot provide the C++ aliases. - On glibc systems with GCC 4.3 we have a sequence of nested includes -> -> -> . In this situation, some of the functions are not yet declared, therefore we cannot provide the C++ aliases. */ # @INCLUDE_NEXT@ @NEXT_SIGNAL_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_SIGNAL_H #define _GL_ALREADY_INCLUDING_SIGNAL_H /* Define pid_t, uid_t. Also, mingw defines sigset_t not in , but in . On Solaris 10, includes , which eventually includes us; so include now, before the second inclusion guard. */ #include /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_SIGNAL_H@ #undef _GL_ALREADY_INCLUDING_SIGNAL_H #ifndef _@GUARD_PREFIX@_SIGNAL_H #define _@GUARD_PREFIX@_SIGNAL_H /* Mac OS X 10.3, FreeBSD 6.4, OpenBSD 3.8, OSF/1 4.0, Solaris 2.6, Android declare pthread_sigmask in , not in . But avoid namespace pollution on glibc systems.*/ #if (@GNULIB_PTHREAD_SIGMASK@ || defined GNULIB_POSIXCHECK) \ && ((defined __APPLE__ && defined __MACH__) \ || defined __FreeBSD__ || defined __OpenBSD__ || defined __osf__ \ || defined __sun || defined __ANDROID__) \ && ! defined __GLIBC__ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* On AIX, sig_atomic_t already includes volatile. C99 requires that 'volatile sig_atomic_t' ignore the extra modifier, but C89 did not. Hence, redefine this to a non-volatile type as needed. */ #if ! @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ # if !GNULIB_defined_sig_atomic_t typedef int rpl_sig_atomic_t; # undef sig_atomic_t # define sig_atomic_t rpl_sig_atomic_t # define GNULIB_defined_sig_atomic_t 1 # endif #endif /* A set or mask of signals. */ #if !@HAVE_SIGSET_T@ # if !GNULIB_defined_sigset_t typedef unsigned int sigset_t; # define GNULIB_defined_sigset_t 1 # endif #endif /* Define sighandler_t, the type of signal handlers. A GNU extension. */ #if !@HAVE_SIGHANDLER_T@ # ifdef __cplusplus extern "C" { # endif # if !GNULIB_defined_sighandler_t typedef void (*sighandler_t) (int); # define GNULIB_defined_sighandler_t 1 # endif # ifdef __cplusplus } # endif #endif #if @GNULIB_SIGNAL_H_SIGPIPE@ # ifndef SIGPIPE /* Define SIGPIPE to a value that does not overlap with other signals. */ # define SIGPIPE 13 # define GNULIB_defined_SIGPIPE 1 /* To actually use SIGPIPE, you also need the gnulib modules 'sigprocmask', 'write', 'stdio'. */ # endif #endif /* Maximum signal number + 1. */ #ifndef NSIG # if defined __TANDEM # define NSIG 32 # endif #endif #if @GNULIB_PTHREAD_SIGMASK@ # if @REPLACE_PTHREAD_SIGMASK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef pthread_sigmask # define pthread_sigmask rpl_pthread_sigmask # endif _GL_FUNCDECL_RPL (pthread_sigmask, int, (int how, const sigset_t *new_mask, sigset_t *old_mask)); _GL_CXXALIAS_RPL (pthread_sigmask, int, (int how, const sigset_t *new_mask, sigset_t *old_mask)); # else # if !@HAVE_PTHREAD_SIGMASK@ _GL_FUNCDECL_SYS (pthread_sigmask, int, (int how, const sigset_t *new_mask, sigset_t *old_mask)); # endif _GL_CXXALIAS_SYS (pthread_sigmask, int, (int how, const sigset_t *new_mask, sigset_t *old_mask)); # endif _GL_CXXALIASWARN (pthread_sigmask); #elif defined GNULIB_POSIXCHECK # undef pthread_sigmask # if HAVE_RAW_DECL_PTHREAD_SIGMASK _GL_WARN_ON_USE (pthread_sigmask, "pthread_sigmask is not portable - " "use gnulib module pthread_sigmask for portability"); # endif #endif #if @GNULIB_RAISE@ # if @REPLACE_RAISE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef raise # define raise rpl_raise # endif _GL_FUNCDECL_RPL (raise, int, (int sig)); _GL_CXXALIAS_RPL (raise, int, (int sig)); # else # if !@HAVE_RAISE@ _GL_FUNCDECL_SYS (raise, int, (int sig)); # endif _GL_CXXALIAS_SYS (raise, int, (int sig)); # endif _GL_CXXALIASWARN (raise); #elif defined GNULIB_POSIXCHECK # undef raise /* Assume raise is always declared. */ _GL_WARN_ON_USE (raise, "raise can crash on native Windows - " "use gnulib module raise for portability"); #endif #if @GNULIB_SIGPROCMASK@ # if !@HAVE_POSIX_SIGNALBLOCKING@ # ifndef GNULIB_defined_signal_blocking # define GNULIB_defined_signal_blocking 1 # endif /* Maximum signal number + 1. */ # ifndef NSIG # define NSIG 32 # endif /* This code supports only 32 signals. */ # if !GNULIB_defined_verify_NSIG_constraint typedef int verify_NSIG_constraint[NSIG <= 32 ? 1 : -1]; # define GNULIB_defined_verify_NSIG_constraint 1 # endif # endif /* When also using extern inline, suppress the use of static inline in standard headers of problematic Apple configurations, as Libc at least through Libc-825.26 (2013-04-09) mishandles it; see, e.g., . Perhaps Apple will fix this some day. */ #if (defined _GL_EXTERN_INLINE_IN_USE && defined __APPLE__ \ && (defined __i386__ || defined __x86_64__)) # undef sigaddset # undef sigdelset # undef sigemptyset # undef sigfillset # undef sigismember #endif /* Test whether a given signal is contained in a signal set. */ # if @HAVE_POSIX_SIGNALBLOCKING@ /* This function is defined as a macro on Mac OS X. */ # if defined __cplusplus && defined GNULIB_NAMESPACE # undef sigismember # endif # else _GL_FUNCDECL_SYS (sigismember, int, (const sigset_t *set, int sig) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (sigismember, int, (const sigset_t *set, int sig)); _GL_CXXALIASWARN (sigismember); /* Initialize a signal set to the empty set. */ # if @HAVE_POSIX_SIGNALBLOCKING@ /* This function is defined as a macro on Mac OS X. */ # if defined __cplusplus && defined GNULIB_NAMESPACE # undef sigemptyset # endif # else _GL_FUNCDECL_SYS (sigemptyset, int, (sigset_t *set) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (sigemptyset, int, (sigset_t *set)); _GL_CXXALIASWARN (sigemptyset); /* Add a signal to a signal set. */ # if @HAVE_POSIX_SIGNALBLOCKING@ /* This function is defined as a macro on Mac OS X. */ # if defined __cplusplus && defined GNULIB_NAMESPACE # undef sigaddset # endif # else _GL_FUNCDECL_SYS (sigaddset, int, (sigset_t *set, int sig) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (sigaddset, int, (sigset_t *set, int sig)); _GL_CXXALIASWARN (sigaddset); /* Remove a signal from a signal set. */ # if @HAVE_POSIX_SIGNALBLOCKING@ /* This function is defined as a macro on Mac OS X. */ # if defined __cplusplus && defined GNULIB_NAMESPACE # undef sigdelset # endif # else _GL_FUNCDECL_SYS (sigdelset, int, (sigset_t *set, int sig) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (sigdelset, int, (sigset_t *set, int sig)); _GL_CXXALIASWARN (sigdelset); /* Fill a signal set with all possible signals. */ # if @HAVE_POSIX_SIGNALBLOCKING@ /* This function is defined as a macro on Mac OS X. */ # if defined __cplusplus && defined GNULIB_NAMESPACE # undef sigfillset # endif # else _GL_FUNCDECL_SYS (sigfillset, int, (sigset_t *set) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (sigfillset, int, (sigset_t *set)); _GL_CXXALIASWARN (sigfillset); /* Return the set of those blocked signals that are pending. */ # if !@HAVE_POSIX_SIGNALBLOCKING@ _GL_FUNCDECL_SYS (sigpending, int, (sigset_t *set) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (sigpending, int, (sigset_t *set)); _GL_CXXALIASWARN (sigpending); /* If OLD_SET is not NULL, put the current set of blocked signals in *OLD_SET. Then, if SET is not NULL, affect the current set of blocked signals by combining it with *SET as indicated in OPERATION. In this implementation, you are not allowed to change a signal handler while the signal is blocked. */ # if !@HAVE_POSIX_SIGNALBLOCKING@ # define SIG_BLOCK 0 /* blocked_set = blocked_set | *set; */ # define SIG_SETMASK 1 /* blocked_set = *set; */ # define SIG_UNBLOCK 2 /* blocked_set = blocked_set & ~*set; */ _GL_FUNCDECL_SYS (sigprocmask, int, (int operation, const sigset_t *set, sigset_t *old_set)); # endif _GL_CXXALIAS_SYS (sigprocmask, int, (int operation, const sigset_t *set, sigset_t *old_set)); _GL_CXXALIASWARN (sigprocmask); /* Install the handler FUNC for signal SIG, and return the previous handler. */ # ifdef __cplusplus extern "C" { # endif # if !GNULIB_defined_function_taking_int_returning_void_t typedef void (*_gl_function_taking_int_returning_void_t) (int); # define GNULIB_defined_function_taking_int_returning_void_t 1 # endif # ifdef __cplusplus } # endif # if !@HAVE_POSIX_SIGNALBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define signal rpl_signal # endif _GL_FUNCDECL_RPL (signal, _gl_function_taking_int_returning_void_t, (int sig, _gl_function_taking_int_returning_void_t func)); _GL_CXXALIAS_RPL (signal, _gl_function_taking_int_returning_void_t, (int sig, _gl_function_taking_int_returning_void_t func)); # else _GL_CXXALIAS_SYS (signal, _gl_function_taking_int_returning_void_t, (int sig, _gl_function_taking_int_returning_void_t func)); # endif _GL_CXXALIASWARN (signal); # if !@HAVE_POSIX_SIGNALBLOCKING@ && GNULIB_defined_SIGPIPE /* Raise signal SIGPIPE. */ _GL_EXTERN_C int _gl_raise_SIGPIPE (void); # endif #elif defined GNULIB_POSIXCHECK # undef sigaddset # if HAVE_RAW_DECL_SIGADDSET _GL_WARN_ON_USE (sigaddset, "sigaddset is unportable - " "use the gnulib module sigprocmask for portability"); # endif # undef sigdelset # if HAVE_RAW_DECL_SIGDELSET _GL_WARN_ON_USE (sigdelset, "sigdelset is unportable - " "use the gnulib module sigprocmask for portability"); # endif # undef sigemptyset # if HAVE_RAW_DECL_SIGEMPTYSET _GL_WARN_ON_USE (sigemptyset, "sigemptyset is unportable - " "use the gnulib module sigprocmask for portability"); # endif # undef sigfillset # if HAVE_RAW_DECL_SIGFILLSET _GL_WARN_ON_USE (sigfillset, "sigfillset is unportable - " "use the gnulib module sigprocmask for portability"); # endif # undef sigismember # if HAVE_RAW_DECL_SIGISMEMBER _GL_WARN_ON_USE (sigismember, "sigismember is unportable - " "use the gnulib module sigprocmask for portability"); # endif # undef sigpending # if HAVE_RAW_DECL_SIGPENDING _GL_WARN_ON_USE (sigpending, "sigpending is unportable - " "use the gnulib module sigprocmask for portability"); # endif # undef sigprocmask # if HAVE_RAW_DECL_SIGPROCMASK _GL_WARN_ON_USE (sigprocmask, "sigprocmask is unportable - " "use the gnulib module sigprocmask for portability"); # endif #endif /* @GNULIB_SIGPROCMASK@ */ #if @GNULIB_SIGACTION@ # if !@HAVE_SIGACTION@ # if !@HAVE_SIGINFO_T@ # if !GNULIB_defined_siginfo_types /* Present to allow compilation, but unsupported by gnulib. */ union sigval { int sival_int; void *sival_ptr; }; /* Present to allow compilation, but unsupported by gnulib. */ struct siginfo_t { int si_signo; int si_code; int si_errno; pid_t si_pid; uid_t si_uid; void *si_addr; int si_status; long si_band; union sigval si_value; }; typedef struct siginfo_t siginfo_t; # define GNULIB_defined_siginfo_types 1 # endif # endif /* !@HAVE_SIGINFO_T@ */ /* We assume that platforms which lack the sigaction() function also lack the 'struct sigaction' type, and vice versa. */ # if !GNULIB_defined_struct_sigaction struct sigaction { union { void (*_sa_handler) (int); /* Present to allow compilation, but unsupported by gnulib. POSIX says that implementations may, but not must, make sa_sigaction overlap with sa_handler, but we know of no implementation where they do not overlap. */ void (*_sa_sigaction) (int, siginfo_t *, void *); } _sa_func; sigset_t sa_mask; /* Not all POSIX flags are supported. */ int sa_flags; }; # define sa_handler _sa_func._sa_handler # define sa_sigaction _sa_func._sa_sigaction /* Unsupported flags are not present. */ # define SA_RESETHAND 1 # define SA_NODEFER 2 # define SA_RESTART 4 # define GNULIB_defined_struct_sigaction 1 # endif _GL_FUNCDECL_SYS (sigaction, int, (int, const struct sigaction *restrict, struct sigaction *restrict)); # elif !@HAVE_STRUCT_SIGACTION_SA_SIGACTION@ # define sa_sigaction sa_handler # endif /* !@HAVE_SIGACTION@, !@HAVE_STRUCT_SIGACTION_SA_SIGACTION@ */ _GL_CXXALIAS_SYS (sigaction, int, (int, const struct sigaction *restrict, struct sigaction *restrict)); _GL_CXXALIASWARN (sigaction); #elif defined GNULIB_POSIXCHECK # undef sigaction # if HAVE_RAW_DECL_SIGACTION _GL_WARN_ON_USE (sigaction, "sigaction is unportable - " "use the gnulib module sigaction for portability"); # endif #endif /* Some systems don't have SA_NODEFER. */ #ifndef SA_NODEFER # define SA_NODEFER 0 #endif #endif /* _@GUARD_PREFIX@_SIGNAL_H */ #endif /* _@GUARD_PREFIX@_SIGNAL_H */ #endif gnuastro-0.5/bootstrapped/tests/sig-handler.h0000644000175000017500000000360013217200023016344 00000000000000/* Convenience declarations when working with . Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_SIG_HANDLER_H #define _GL_SIG_HANDLER_H #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef SIG_HANDLER_INLINE # define SIG_HANDLER_INLINE _GL_INLINE #endif /* Convenience type when working with signal handlers. */ typedef void (*sa_handler_t) (int); /* Return the handler of a signal, as a sa_handler_t value regardless of its true type. The resulting function can be compared to special values like SIG_IGN but it is not portable to call it. */ SIG_HANDLER_INLINE sa_handler_t _GL_ATTRIBUTE_PURE get_handler (struct sigaction const *a) { #ifdef SA_SIGINFO /* POSIX says that special values like SIG_IGN can only occur when action.sa_flags does not contain SA_SIGINFO. But in Linux 2.4, for example, sa_sigaction and sa_handler are aliases and a signal is ignored if sa_sigaction (after casting) equals SIG_IGN. So use (and cast) sa_sigaction in that case. */ if (a->sa_flags & SA_SIGINFO) return (sa_handler_t) a->sa_sigaction; #endif return a->sa_handler; } _GL_INLINE_HEADER_END #endif /* _GL_SIG_HANDLER_H */ gnuastro-0.5/bootstrapped/tests/test-setlocale2.sh0000755000175000017500000000133713217200024017355 00000000000000#!/bin/sh # Test locale names with likely unsupported encoding in Unix syntax. for name in ar_SA.ISO-8859-1 fr_FR.CP1251 zh_TW.GB18030 zh_CN.BIG5; do env LC_ALL=$name ./test-setlocale2${EXEEXT} 1 || exit 1 done # Test locale names with likely unsupported encoding in native Windows syntax. for name in "Arabic_Saudi Arabia.1252" "Arabic_Saudi Arabia.65001" \ French_France.65001 Japanese_Japan.65001 Turkish_Turkey.65001 \ Chinese_Taiwan.65001 Chinese_China.54936 Chinese_China.65001; do # Here we use 'env' to set the LC_ALL environment variable, because on # Solaris 11.0, the /bin/sh refuses to do it for Turkish_Turkey.65001. env LC_ALL="$name" ./test-setlocale2${EXEEXT} 1 || exit 1 done exit 0 gnuastro-0.5/bootstrapped/tests/test-setlocale1.sh0000755000175000017500000000150613217200024017352 00000000000000#!/bin/sh : ${LOCALE_FR=fr_FR} : ${LOCALE_FR_UTF8=fr_FR.UTF-8} : ${LOCALE_JA=ja_JP} : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_FR = none && test $LOCALE_FR_UTF8 = none \ && test $LOCALE_JA = none && test $LOCALE_ZH_CN = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no locale for testing is installed" else echo "Skipping test: no locale for testing is supported" fi exit 77 fi if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR ./test-setlocale1${EXEEXT} || exit 1 fi if test $LOCALE_FR_UTF8 != none; then LC_ALL=$LOCALE_FR_UTF8 ./test-setlocale1${EXEEXT} || exit 1 fi if test $LOCALE_JA != none; then LC_ALL=$LOCALE_JA ./test-setlocale1${EXEEXT} || exit 1 fi if test $LOCALE_ZH_CN != none; then LC_ALL=$LOCALE_ZH_CN ./test-setlocale1${EXEEXT} || exit 1 fi exit 0 gnuastro-0.5/bootstrapped/tests/test-select-out.sh0000755000175000017500000000157013217200024017403 00000000000000#!/bin/sh # Test select() on file descriptors opened for writing. tmpfiles="" trap 'rm -fr $tmpfiles' 1 2 3 15 tmpfiles="$tmpfiles t-select-out.out t-select-out.tmp" # Regular files. rm -f t-select-out.tmp ./test-select-fd${EXEEXT} w 1 t-select-out.tmp > t-select-out.out test `cat t-select-out.tmp` = "1" || exit 1 # Pipes. if false; then # This test fails on some platforms. rm -f t-select-out.tmp ( { echo abc; ./test-select-fd${EXEEXT} w 1 t-select-out.tmp; } | { sleep 1; cat; } ) > /dev/null test `cat t-select-out.tmp` = "0" || exit 1 fi rm -f t-select-out.tmp ( { sleep 1; echo abc; ./test-select-fd${EXEEXT} w 1 t-select-out.tmp; } | cat) > /dev/null test `cat t-select-out.tmp` = "1" || exit 1 # Special files. rm -f t-select-out.tmp ./test-select-fd${EXEEXT} w 1 t-select-out.tmp > /dev/null test `cat t-select-out.tmp` = "1" || exit 1 rm -fr $tmpfiles exit 0 gnuastro-0.5/bootstrapped/tests/test-select-in.sh0000755000175000017500000000166113217200024017203 00000000000000#!/bin/sh # Test select() on file descriptors opened for reading. # This test is known to fail on Solaris 2.6 and older, due to its handling # of /dev/null. tmpfiles="" trap 'rm -fr $tmpfiles' 1 2 3 15 tmpfiles="$tmpfiles t-select-in.tmp" # Regular files. rm -f t-select-in.tmp ./test-select-fd${EXEEXT} r 0 t-select-in.tmp < ./test-select-fd${EXEEXT} test `cat t-select-in.tmp` = "1" || exit 1 # Pipes. rm -f t-select-in.tmp { sleep 1; echo abc; } | \ { ./test-select-fd${EXEEXT} r 0 t-select-in.tmp; cat > /dev/null; } test `cat t-select-in.tmp` = "0" || exit 1 rm -f t-select-in.tmp echo abc | { sleep 1; ./test-select-fd${EXEEXT} r 0 t-select-in.tmp; } test `cat t-select-in.tmp` = "1" || exit 1 # Special files. # This part of the test is known to fail on Solaris 2.6 and older. rm -f t-select-in.tmp ./test-select-fd${EXEEXT} r 0 t-select-in.tmp < /dev/null test `cat t-select-in.tmp` = "1" || exit 1 rm -fr $tmpfiles exit 0 gnuastro-0.5/bootstrapped/tests/test-select.h0000644000175000017500000002615713217200024016420 00000000000000/* Test of select() substitute. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini, 2008. */ #include #include #include #include #include #include #include #include #include #include #include "macros.h" #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WINDOWS_NATIVE #endif #ifdef HAVE_SYS_WAIT_H # include #endif #ifndef SO_REUSEPORT # define SO_REUSEPORT SO_REUSEADDR #endif #define TEST_PORT 12345 typedef int (*select_fn) (int, fd_set *, fd_set *, fd_set *, struct timeval *); /* Minimal testing infrastructure. */ static int failures; static void failed (const char *reason) { if (++failures > 1) printf (" "); printf ("failed (%s)\n", reason); } static int test (void (*fn) (select_fn), select_fn my_select, const char *msg) { failures = 0; printf ("%s... ", msg); fflush (stdout); fn (my_select); if (!failures) printf ("passed\n"); return failures; } /* Funny socket code. */ static int open_server_socket (void) { int s, x; struct sockaddr_in ia; s = socket (AF_INET, SOCK_STREAM, 0); x = 1; setsockopt (s, SOL_SOCKET, SO_REUSEPORT, &x, sizeof (x)); memset (&ia, 0, sizeof (ia)); ia.sin_family = AF_INET; inet_pton (AF_INET, "127.0.0.1", &ia.sin_addr); ia.sin_port = htons (TEST_PORT); if (bind (s, (struct sockaddr *) &ia, sizeof (ia)) < 0) { perror ("bind"); exit (77); } if (listen (s, 1) < 0) { perror ("listen"); exit (77); } return s; } static int connect_to_socket (bool blocking) { int s; struct sockaddr_in ia; s = socket (AF_INET, SOCK_STREAM, 0); memset (&ia, 0, sizeof (ia)); ia.sin_family = AF_INET; inet_pton (AF_INET, "127.0.0.1", &ia.sin_addr); ia.sin_port = htons (TEST_PORT); if (!blocking) { #ifdef WINDOWS_NATIVE unsigned long iMode = 1; ioctl (s, FIONBIO, (char *) &iMode); #elif defined F_GETFL int oldflags = fcntl (s, F_GETFL, NULL); if (!(oldflags & O_NONBLOCK)) fcntl (s, F_SETFL, oldflags | O_NONBLOCK); #endif } if (connect (s, (struct sockaddr *) &ia, sizeof (ia)) < 0 && (blocking || errno != EINPROGRESS)) { perror ("connect"); exit (77); } return s; } /* A slightly more convenient interface to select(2). Waits until a specific event occurs on a file descriptor FD. EV is a bit mask of events to look for: SEL_IN - input can be polled without blocking, SEL_OUT - output can be provided without blocking, SEL_EXC - an exception occurred, A maximum wait time is specified by TIMEOUT. *TIMEOUT = { 0, 0 } means to return immediately, TIMEOUT = NULL means to wait indefinitely. */ enum { SEL_IN = 1, SEL_OUT = 2, SEL_EXC = 4 }; static int do_select (int fd, int ev, struct timeval *timeout, select_fn my_select) { fd_set rfds, wfds, xfds; int r, rev; FD_ZERO (&rfds); FD_ZERO (&wfds); FD_ZERO (&xfds); if (ev & SEL_IN) FD_SET (fd, &rfds); if (ev & SEL_OUT) FD_SET (fd, &wfds); if (ev & SEL_EXC) FD_SET (fd, &xfds); r = my_select (fd + 1, &rfds, &wfds, &xfds, timeout); if (r < 0) return r; rev = 0; if (FD_ISSET (fd, &rfds)) rev |= SEL_IN; if (FD_ISSET (fd, &wfds)) rev |= SEL_OUT; if (FD_ISSET (fd, &xfds)) rev |= SEL_EXC; if (rev && r == 0) failed ("select returned 0"); if (rev & ~ev) failed ("select returned unrequested events"); return rev; } static int do_select_nowait (int fd, int ev, select_fn my_select) { struct timeval tv0; tv0.tv_sec = 0; tv0.tv_usec = 0; return do_select (fd, ev, &tv0, my_select); } static int do_select_wait (int fd, int ev, select_fn my_select) { return do_select (fd, ev, NULL, my_select); } /* Test select(2) for TTYs. */ #ifdef INTERACTIVE static void test_tty (select_fn my_select) { if (do_select_nowait (0, SEL_IN, my_select) != 0) failed ("can read"); if (do_select_nowait (0, SEL_OUT, my_select) == 0) failed ("cannot write"); if (do_select_wait (0, SEL_IN, my_select) == 0) failed ("return with infinite timeout"); getchar (); if (do_select_nowait (0, SEL_IN, my_select) != 0) failed ("can read after getc"); } #endif static int do_select_bad_nfd_nowait (int nfd, select_fn my_select) { struct timeval tv0; tv0.tv_sec = 0; tv0.tv_usec = 0; errno = 0; return my_select (nfd, NULL, NULL, NULL, &tv0); } static void test_bad_nfd (select_fn my_select) { if (do_select_bad_nfd_nowait (-1, my_select) != -1 || errno != EINVAL) failed ("invalid errno after negative nfds"); /* Can't test FD_SETSIZE + 1 for EINVAL, since some systems allow dynamically larger set size by redefining FD_SETSIZE anywhere up to the actual maximum fd. */ /* if (do_select_bad_nfd_nowait (FD_SETSIZE + 1, my_select) != -1 */ /* || errno != EINVAL) */ /* failed ("invalid errno after bogus nfds"); */ } /* Test select(2) on invalid file descriptors. */ static int do_select_bad_fd (int fd, int ev, struct timeval *timeout, select_fn my_select) { fd_set rfds, wfds, xfds; FD_ZERO (&rfds); FD_ZERO (&wfds); FD_ZERO (&xfds); if (ev & SEL_IN) FD_SET (fd, &rfds); if (ev & SEL_OUT) FD_SET (fd, &wfds); if (ev & SEL_EXC) FD_SET (fd, &xfds); errno = 0; return my_select (fd + 1, &rfds, &wfds, &xfds, timeout); /* In this case, when fd is invalid, on some platforms, the bit for fd is left alone in the fd_set, whereas on other platforms it is cleared. So, don't check the bit for fd here. */ } static int do_select_bad_fd_nowait (int fd, int ev, select_fn my_select) { struct timeval tv0; tv0.tv_sec = 0; tv0.tv_usec = 0; return do_select_bad_fd (fd, ev, &tv0, my_select); } static void test_bad_fd (select_fn my_select) { /* This tests fails on OSF/1 and native Windows, even with fd = 16. */ #if !(defined __osf__ || defined WINDOWS_NATIVE) int fd; /* On Linux, Mac OS X, *BSD, values of fd like 99 or 399 are discarded by the kernel early and therefore do *not* lead to EBADF, as required by POSIX. */ # if defined __linux__ || (defined __APPLE__ && defined __MACH__) || (defined __FreeBSD__ || defined __DragonFly__) || defined __OpenBSD__ || defined __NetBSD__ fd = 14; # else fd = 99; # endif close (fd); if (do_select_bad_fd_nowait (fd, SEL_IN, my_select) == 0 || errno != EBADF) failed ("invalid fd among rfds"); if (do_select_bad_fd_nowait (fd, SEL_OUT, my_select) == 0 || errno != EBADF) failed ("invalid fd among wfds"); if (do_select_bad_fd_nowait (fd, SEL_EXC, my_select) == 0 || errno != EBADF) failed ("invalid fd among xfds"); #endif } /* Test select(2) for unconnected nonblocking sockets. */ static void test_connect_first (select_fn my_select) { int s = open_server_socket (); struct sockaddr_in ia; socklen_t addrlen; int c1, c2; if (do_select_nowait (s, SEL_IN | SEL_EXC, my_select) != 0) failed ("can read, socket not connected"); c1 = connect_to_socket (false); if (do_select_wait (s, SEL_IN | SEL_EXC, my_select) != SEL_IN) failed ("expecting readability on passive socket"); if (do_select_nowait (s, SEL_IN | SEL_EXC, my_select) != SEL_IN) failed ("expecting readability on passive socket"); addrlen = sizeof (ia); c2 = accept (s, (struct sockaddr *) &ia, &addrlen); ASSERT (close (s) == 0); ASSERT (close (c1) == 0); ASSERT (close (c2) == 0); } /* Test select(2) for unconnected blocking sockets. */ static void test_accept_first (select_fn my_select) { #ifndef WINDOWS_NATIVE int s = open_server_socket (); struct sockaddr_in ia; socklen_t addrlen; char buf[3]; int c, pid; pid = fork (); if (pid < 0) return; if (pid == 0) { addrlen = sizeof (ia); c = accept (s, (struct sockaddr *) &ia, &addrlen); ASSERT (close (s) == 0); ASSERT (write (c, "foo", 3) == 3); ASSERT (read (c, buf, 3) == 3); shutdown (c, SHUT_RD); ASSERT (close (c) == 0); exit (0); } else { ASSERT (close (s) == 0); c = connect_to_socket (true); if (do_select_nowait (c, SEL_OUT, my_select) != SEL_OUT) failed ("cannot write after blocking connect"); ASSERT (write (c, "foo", 3) == 3); wait (&pid); if (do_select_wait (c, SEL_IN, my_select) != SEL_IN) failed ("cannot read data left in the socket by closed process"); ASSERT (read (c, buf, 3) == 3); ASSERT (write (c, "foo", 3) == 3); (void) close (c); /* may fail with errno = ECONNRESET */ } #endif } /* Common code for pipes and connected sockets. */ static void test_pair (int rd, int wd, select_fn my_select) { char buf[3]; if (do_select_wait (wd, SEL_IN | SEL_OUT | SEL_EXC, my_select) != SEL_OUT) failed ("expecting writability before writing"); if (do_select_nowait (wd, SEL_IN | SEL_OUT | SEL_EXC, my_select) != SEL_OUT) failed ("expecting writability before writing"); ASSERT (write (wd, "foo", 3) == 3); if (do_select_wait (rd, SEL_IN, my_select) != SEL_IN) failed ("expecting readability after writing"); if (do_select_nowait (rd, SEL_IN, my_select) != SEL_IN) failed ("expecting readability after writing"); ASSERT (read (rd, buf, 3) == 3); } /* Test select(2) on connected sockets. */ static void test_socket_pair (select_fn my_select) { struct sockaddr_in ia; socklen_t addrlen = sizeof (ia); int s = open_server_socket (); int c1 = connect_to_socket (false); int c2 = accept (s, (struct sockaddr *) &ia, &addrlen); ASSERT (close (s) == 0); test_pair (c1, c2, my_select); ASSERT (close (c1) == 0); ASSERT (write (c2, "foo", 3) == 3); (void) close (c2); /* may fail with errno = ECONNRESET */ } /* Test select(2) on pipes. */ static void test_pipe (select_fn my_select) { int fd[2]; ASSERT (pipe (fd) == 0); test_pair (fd[0], fd[1], my_select); ASSERT (close (fd[0]) == 0); ASSERT (close (fd[1]) == 0); } /* Do them all. */ static int test_function (select_fn my_select) { int result = 0; #ifdef INTERACTIVE printf ("Please press Enter\n"); test (test_tty, "TTY", my_select); #endif result += test (test_bad_nfd, my_select, "Invalid nfd test"); result += test (test_bad_fd, my_select, "Invalid fd test"); result += test (test_connect_first, my_select, "Unconnected socket test"); result += test (test_socket_pair, my_select, "Connected sockets test"); result += test (test_accept_first, my_select, "General socket test with fork"); result += test (test_pipe, my_select, "Pipe test"); return result; } gnuastro-0.5/bootstrapped/tests/same-inode.h0000644000175000017500000000324513217200023016175 00000000000000/* Determine whether two stat buffers are known to refer to the same file. Copyright (C) 2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef SAME_INODE_H # define SAME_INODE_H 1 # include # if defined __VMS && __CRTL_VER < 80200000 # define SAME_INODE(a, b) \ ((a).st_ino[0] == (b).st_ino[0] \ && (a).st_ino[1] == (b).st_ino[1] \ && (a).st_ino[2] == (b).st_ino[2] \ && (a).st_dev == (b).st_dev) # elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Native Windows. */ # if _GL_WINDOWS_STAT_INODES /* stat() and fstat() set st_dev and st_ino to 0 if information about the inode is not available. */ # define SAME_INODE(a, b) \ (!((a).st_ino == 0 && (a).st_dev == 0) \ && (a).st_ino == (b).st_ino && (a).st_dev == (b).st_dev) # else /* stat() and fstat() set st_ino to 0 always. */ # define SAME_INODE(a, b) 0 # endif # else # define SAME_INODE(a, b) \ ((a).st_ino == (b).st_ino \ && (a).st_dev == (b).st_dev) # endif #endif gnuastro-0.5/bootstrapped/tests/test-perror.sh0000755000175000017500000000170313217200024016626 00000000000000#!/bin/sh : ${srcdir=.} . "$srcdir/init.sh"; path_prepend_ . # Test NULL prefix. Result should not contain a number, except in lines that # start with 'EDC' (IBM z/OS libc produces an error identifier before the # error message). test-perror 2>&1 >/dev/null | LC_ALL=C tr -d '\r' > t-perror.tmp grep -v '^EDC' t-perror.tmp | grep '[0-9]' > /dev/null \ && fail_ "result should not contain a number" # Test empty prefix. Result should be the same. test-perror '' 2>&1 >/dev/null | LC_ALL=C tr -d '\r' > t-perror1.tmp diff t-perror.tmp t-perror1.tmp \ || fail_ "empty prefix should behave like NULL argument" # Test non-empty prefix. test-perror foo 2>&1 >/dev/null | LC_ALL=C tr -d '\r' > t-perror3.tmp sed -e 's/^/foo: /' < t-perror.tmp > t-perror2.tmp diff t-perror2.tmp t-perror3.tmp || fail_ "prefix applied incorrectly" # Test exit status. test-perror >out 2>/dev/null || fail_ "unexpected exit status" test -s out && fail_ "unexpected output" Exit 0 gnuastro-0.5/bootstrapped/tests/pathmax.h0000644000175000017500000000554713217200023015625 00000000000000/* Define PATH_MAX somehow. Requires sys/types.h. Copyright (C) 1992, 1999, 2001, 2003, 2005, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _PATHMAX_H # define _PATHMAX_H /* POSIX:2008 defines PATH_MAX to be the maximum number of bytes in a filename, including the terminating NUL byte. PATH_MAX is not defined on systems which have no limit on filename length, such as GNU/Hurd. This file does *not* define PATH_MAX always. Programs that use this file can handle the GNU/Hurd case in several ways: - Either with a package-wide handling, or with a per-file handling, - Either through a #ifdef PATH_MAX or through a fallback like #ifndef PATH_MAX # define PATH_MAX 8192 #endif or through a fallback like #ifndef PATH_MAX # define PATH_MAX pathconf ("/", _PC_PATH_MAX) #endif */ # include # include # ifndef _POSIX_PATH_MAX # define _POSIX_PATH_MAX 256 # endif /* Don't include sys/param.h if it already has been. */ # if defined HAVE_SYS_PARAM_H && !defined PATH_MAX && !defined MAXPATHLEN # include # endif # if !defined PATH_MAX && defined MAXPATHLEN # define PATH_MAX MAXPATHLEN # endif # ifdef __hpux /* On HP-UX, PATH_MAX designates the maximum number of bytes in a filename, *not* including the terminating NUL byte, and is set to 1023. Additionally, when _XOPEN_SOURCE is defined to 500 or more, PATH_MAX is not defined at all any more. */ # undef PATH_MAX # define PATH_MAX 1024 # endif # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* The page "Naming Files, Paths, and Namespaces" on msdn.microsoft.com, section "Maximum Path Length Limitation", explains that the maximum size of a filename, including the terminating NUL byte, is 260 = 3 + 256 + 1. This is the same value as - FILENAME_MAX in , - _MAX_PATH in , - MAX_PATH in . Undefine the original value, because mingw's gets it wrong. */ # undef PATH_MAX # define PATH_MAX 260 # endif #endif /* _PATHMAX_H */ gnuastro-0.5/bootstrapped/tests/test-open.h0000644000175000017500000000646113217200024016076 00000000000000/* Test of opening a file descriptor. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ /* Make test_open always inline if we're using Fortify, which defines __always_inline to do that. Do nothing otherwise. This works around a glibc bug whereby 'open' cannot be used as a function pointer when _FORTIFY_SOURCE is positive. */ #if __GLIBC__ && defined __always_inline # define ALWAYS_INLINE __always_inline #else # define ALWAYS_INLINE #endif /* This file is designed to test both open(n,buf[,mode]) and openat(AT_FDCWD,n,buf[,mode]). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static ALWAYS_INLINE int test_open (int (*func) (char const *, int, ...), bool print) { int fd; /* Remove anything from prior partial run. */ unlink (BASE "file"); /* Cannot create directory. */ errno = 0; ASSERT (func ("nonexist.ent/", O_CREAT | O_RDONLY, 0600) == -1); ASSERT (errno == ENOTDIR || errno == EISDIR || errno == ENOENT || errno == EINVAL); /* Create a regular file. */ fd = func (BASE "file", O_CREAT | O_RDONLY, 0600); ASSERT (0 <= fd); ASSERT (close (fd) == 0); /* Trailing slash handling. */ errno = 0; ASSERT (func (BASE "file/", O_RDONLY) == -1); ASSERT (errno == ENOTDIR || errno == EISDIR || errno == EINVAL); /* Directories cannot be opened for writing. */ errno = 0; ASSERT (func (".", O_WRONLY) == -1); ASSERT (errno == EISDIR || errno == EACCES); /* /dev/null must exist, and be writable. */ fd = func ("/dev/null", O_RDONLY); ASSERT (0 <= fd); { char c; ASSERT (read (fd, &c, 1) == 0); } ASSERT (close (fd) == 0); fd = func ("/dev/null", O_WRONLY); ASSERT (0 <= fd); ASSERT (write (fd, "c", 1) == 1); ASSERT (close (fd) == 0); /* Although O_NONBLOCK on regular files can be ignored, it must not cause a failure. */ fd = func (BASE "file", O_NONBLOCK | O_RDONLY); ASSERT (0 <= fd); ASSERT (close (fd) == 0); /* Symlink handling, where supported. */ if (symlink (BASE "file", BASE "link") != 0) { ASSERT (unlink (BASE "file") == 0); if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } errno = 0; ASSERT (func (BASE "link/", O_RDONLY) == -1); ASSERT (errno == ENOTDIR); fd = func (BASE "link", O_RDONLY); ASSERT (0 <= fd); ASSERT (close (fd) == 0); /* Cleanup. */ ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link") == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-nl_langinfo.sh0000755000175000017500000000066513217200024017611 00000000000000#!/bin/sh LC_ALL=C ./test-nl_langinfo${EXEEXT} 0 || exit 1 # Test whether a specific traditional locale is installed. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR ./test-nl_langinfo${EXEEXT} 1 || exit 1 fi # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 != none; then LC_ALL=$LOCALE_FR_UTF8 ./test-nl_langinfo${EXEEXT} 2 || exit 1 fi exit 0 gnuastro-0.5/bootstrapped/tests/netinet_in.in.h0000644000175000017500000000247513217200023016721 00000000000000/* Substitute for . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_NETINET_IN_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if @HAVE_NETINET_IN_H@ /* On many platforms, assumes prior inclusion of . */ # include /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_NETINET_IN_H@ #endif #ifndef _@GUARD_PREFIX@_NETINET_IN_H #define _@GUARD_PREFIX@_NETINET_IN_H #if !@HAVE_NETINET_IN_H@ /* A platform that lacks . */ # include #endif #endif /* _@GUARD_PREFIX@_NETINET_IN_H */ #endif /* _@GUARD_PREFIX@_NETINET_IN_H */ gnuastro-0.5/bootstrapped/tests/zerosize-ptr.h0000644000175000017500000000471713217200024016637 00000000000000/* Return a pointer to a zero-size object in memory. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* ISO C 99 does not allow memcmp(), memchr() etc. to be invoked with a NULL argument. Therefore this file produces a non-NULL pointer which cannot be dereferenced, if possible. */ #include /* Test whether mmap() and mprotect() are available. We don't use HAVE_MMAP, because AC_FUNC_MMAP would not define it on HP-UX. HAVE_MPROTECT is not enough, because mingw does not have mmap() but has an mprotect() function in libgcc.a. */ #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # include # include # include # include /* Define MAP_FILE when it isn't otherwise. */ # ifndef MAP_FILE # define MAP_FILE 0 # endif #endif /* Return a pointer to a zero-size object in memory (that is, actually, a pointer to a page boundary where the previous page is readable and writable and the next page is neither readable not writable), if possible. Return NULL otherwise. */ static void * zerosize_ptr (void) { /* Use mmap and mprotect when they exist. Don't test HAVE_MMAP, because it is not defined on HP-UX 11 (since it does not support MAP_FIXED). */ #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # if HAVE_MAP_ANONYMOUS const int flags = MAP_ANONYMOUS | MAP_PRIVATE; const int fd = -1; # else /* !HAVE_MAP_ANONYMOUS */ const int flags = MAP_FILE | MAP_PRIVATE; int fd = open ("/dev/zero", O_RDONLY, 0666); if (fd >= 0) # endif { int pagesize = getpagesize (); char *two_pages = (char *) mmap (NULL, 2 * pagesize, PROT_READ | PROT_WRITE, flags, fd, 0); if (two_pages != (char *)(-1) && mprotect (two_pages + pagesize, pagesize, PROT_NONE) == 0) return two_pages + pagesize; } #endif return NULL; } gnuastro-0.5/bootstrapped/tests/test-mbsspn.sh0000755000175000017500000000056513217200024016624 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-mbsspn${EXEEXT} gnuastro-0.5/bootstrapped/tests/test-mbspbrk.sh0000755000175000017500000000056613217200024016763 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-mbspbrk${EXEEXT} gnuastro-0.5/bootstrapped/tests/test-mbsinit.sh0000755000175000017500000000056613217200024016770 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-mbsinit${EXEEXT} gnuastro-0.5/bootstrapped/tests/test-mbschr.sh0000755000175000017500000000056513217200024016600 00000000000000#!/bin/sh # Test whether a specific GB18030 locale is installed. : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_ZH_CN = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no chinese GB18030 locale is installed" else echo "Skipping test: no chinese GB18030 locale is supported" fi exit 77 fi LC_ALL=$LOCALE_ZH_CN \ ./test-mbschr${EXEEXT} gnuastro-0.5/bootstrapped/tests/test-mbrtowc-w32-5.sh0000755000175000017500000000012013217200024017535 00000000000000#!/bin/sh # Test a CP936 locale. ./test-mbrtowc-w32${EXEEXT} Chinese_China 936 gnuastro-0.5/bootstrapped/tests/test-mbrtowc-w32-4.sh0000755000175000017500000000012113217200024017535 00000000000000#!/bin/sh # Test a CP950 locale. ./test-mbrtowc-w32${EXEEXT} Chinese_Taiwan 950 gnuastro-0.5/bootstrapped/tests/test-mbrtowc-w32-3.sh0000755000175000017500000000012113217200024017534 00000000000000#!/bin/sh # Test a CP932 locale. ./test-mbrtowc-w32${EXEEXT} Japanese_Japan 932 gnuastro-0.5/bootstrapped/tests/test-mbrtowc-w32-2.sh0000755000175000017500000000013213217200024017535 00000000000000#!/bin/sh # Test a CP1256 locale. ./test-mbrtowc-w32${EXEEXT} "Arabic_Saudi Arabia" 1256 gnuastro-0.5/bootstrapped/tests/test-mbrtowc-w32-1.sh0000755000175000017500000000012213217200024017533 00000000000000#!/bin/sh # Test a CP1252 locale. ./test-mbrtowc-w32${EXEEXT} French_France 1252 gnuastro-0.5/bootstrapped/tests/test-mbrtowc5.sh0000755000175000017500000000022513217200024017055 00000000000000#!/bin/sh # Test whether the POSIX locale has encoding errors. LC_ALL=C \ ./test-mbrtowc${EXEEXT} 5 || exit LC_ALL=POSIX \ ./test-mbrtowc${EXEEXT} 5 gnuastro-0.5/bootstrapped/tests/test-mbrtowc4.sh0000755000175000017500000000060213217200024017053 00000000000000#!/bin/sh # Test whether a specific GB18030 locale is installed. : ${LOCALE_ZH_CN=zh_CN.GB18030} if test $LOCALE_ZH_CN = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no transitional chinese locale is installed" else echo "Skipping test: no transitional chinese locale is supported" fi exit 77 fi LC_ALL=$LOCALE_ZH_CN \ ./test-mbrtowc${EXEEXT} 4 gnuastro-0.5/bootstrapped/tests/test-mbrtowc3.sh0000755000175000017500000000056013217200024017055 00000000000000#!/bin/sh # Test whether a specific EUC-JP locale is installed. : ${LOCALE_JA=ja_JP} if test $LOCALE_JA = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no traditional japanese locale is installed" else echo "Skipping test: no traditional japanese locale is supported" fi exit 77 fi LC_ALL=$LOCALE_JA \ ./test-mbrtowc${EXEEXT} 3 gnuastro-0.5/bootstrapped/tests/test-mbrtowc2.sh0000755000175000017500000000057013217200024017055 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-mbrtowc${EXEEXT} 2 gnuastro-0.5/bootstrapped/tests/test-mbrtowc1.sh0000755000175000017500000000054513217200024017056 00000000000000#!/bin/sh # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no traditional french locale is installed" else echo "Skipping test: no traditional french locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR \ ./test-mbrtowc${EXEEXT} 1 gnuastro-0.5/bootstrapped/tests/malloca.valgrind0000644000175000017500000000025713217200023017143 00000000000000# Suppress a valgrind message about use of uninitialized memory in freea(). # This use is OK because it provides only a speedup. { freea Memcheck:Cond fun:freea } gnuastro-0.5/bootstrapped/tests/malloca.h0000644000175000017500000001067413217200023015570 00000000000000/* Safe automatic memory allocation. Copyright (C) 2003-2007, 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2003. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MALLOCA_H #define _MALLOCA_H #include #include #include #include #include "xalloc-oversized.h" #ifdef __cplusplus extern "C" { #endif /* safe_alloca(N) is equivalent to alloca(N) when it is safe to call alloca(N); otherwise it returns NULL. It either returns N bytes of memory allocated on the stack, that lasts until the function returns, or NULL. Use of safe_alloca should be avoided: - inside arguments of function calls - undefined behaviour, - in inline functions - the allocation may actually last until the calling function returns. */ #if HAVE_ALLOCA /* The OS usually guarantees only one guard page at the bottom of the stack, and a page size can be as small as 4096 bytes. So we cannot safely allocate anything larger than 4096 bytes. Also care for the possibility of a few compiler-allocated temporary stack slots. This must be a macro, not a function. */ # define safe_alloca(N) ((N) < 4032 ? alloca (N) : NULL) #else # define safe_alloca(N) ((void) (N), NULL) #endif /* malloca(N) is a safe variant of alloca(N). It allocates N bytes of memory allocated on the stack, that must be freed using freea() before the function returns. Upon failure, it returns NULL. */ #if HAVE_ALLOCA # define malloca(N) \ ((N) < 4032 - sa_increment \ ? (void *) ((char *) alloca ((N) + sa_increment) + sa_increment) \ : mmalloca (N)) #else # define malloca(N) \ mmalloca (N) #endif extern void * mmalloca (size_t n); /* Free a block of memory allocated through malloca(). */ #if HAVE_ALLOCA extern void freea (void *p); #else # define freea free #endif /* nmalloca(N,S) is an overflow-safe variant of malloca (N * S). It allocates an array of N objects, each with S bytes of memory, on the stack. S must be positive and N must be nonnegative. The array must be freed using freea() before the function returns. */ #define nmalloca(n, s) (xalloc_oversized (n, s) ? NULL : malloca ((n) * (s))) #ifdef __cplusplus } #endif /* ------------------- Auxiliary, non-public definitions ------------------- */ /* Determine the alignment of a type at compile time. */ #if defined __GNUC__ || defined __IBM__ALIGNOF__ # define sa_alignof __alignof__ #elif defined __cplusplus template struct sa_alignof_helper { char __slot1; type __slot2; }; # define sa_alignof(type) offsetof (sa_alignof_helper, __slot2) #elif defined __hpux /* Work around a HP-UX 10.20 cc bug with enums constants defined as offsetof values. */ # define sa_alignof(type) (sizeof (type) <= 4 ? 4 : 8) #elif defined _AIX /* Work around an AIX 3.2.5 xlc bug with enums constants defined as offsetof values. */ # define sa_alignof(type) (sizeof (type) <= 4 ? 4 : 8) #else # define sa_alignof(type) offsetof (struct { char __slot1; type __slot2; }, __slot2) #endif enum { /* The desired alignment of memory allocations is the maximum alignment among all elementary types. */ sa_alignment_long = sa_alignof (long), sa_alignment_double = sa_alignof (double), #if HAVE_LONG_LONG_INT sa_alignment_longlong = sa_alignof (long long), #endif sa_alignment_longdouble = sa_alignof (long double), sa_alignment_max = ((sa_alignment_long - 1) | (sa_alignment_double - 1) #if HAVE_LONG_LONG_INT | (sa_alignment_longlong - 1) #endif | (sa_alignment_longdouble - 1) ) + 1, /* The increment that guarantees room for a magic word must be >= sizeof (int) and a multiple of sa_alignment_max. */ sa_increment = ((sizeof (int) + sa_alignment_max - 1) / sa_alignment_max) * sa_alignment_max }; #endif /* _MALLOCA_H */ gnuastro-0.5/bootstrapped/tests/test-lstat.h0000644000175000017500000000727113217200024016264 00000000000000/* Test of lstat() function. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson, 2008; and Eric Blake, 2009. */ /* This file is designed to test both lstat(n,buf) and fstatat(AT_FDCWD,n,buf,AT_SYMLINK_NOFOLLOW). FUNC is the function to test. Assumes that BASE and ASSERT are already defined, and that appropriate headers are already included. If PRINT, warn before skipping symlink tests with status 77. */ static int test_lstat_func (int (*func) (char const *, struct stat *), bool print) { struct stat st1; struct stat st2; /* Test for common directories. */ ASSERT (func (".", &st1) == 0); ASSERT (func ("./", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (S_ISDIR (st1.st_mode)); ASSERT (S_ISDIR (st2.st_mode)); ASSERT (func ("/", &st1) == 0); ASSERT (func ("///", &st2) == 0); ASSERT (SAME_INODE (st1, st2)); ASSERT (S_ISDIR (st1.st_mode)); ASSERT (S_ISDIR (st2.st_mode)); ASSERT (func ("..", &st1) == 0); ASSERT (S_ISDIR (st1.st_mode)); /* Test for error conditions. */ errno = 0; ASSERT (func ("", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch", &st1) == -1); ASSERT (errno == ENOENT); errno = 0; ASSERT (func ("nosuch/", &st1) == -1); ASSERT (errno == ENOENT); ASSERT (close (creat (BASE "file", 0600)) == 0); ASSERT (func (BASE "file", &st1) == 0); ASSERT (S_ISREG (st1.st_mode)); errno = 0; ASSERT (func (BASE "file/", &st1) == -1); ASSERT (errno == ENOTDIR); /* Now for some symlink tests, where supported. We set up: link1 -> directory link2 -> file link3 -> dangling link4 -> loop then test behavior both with and without trailing slash. */ if (symlink (".", BASE "link1") != 0) { ASSERT (unlink (BASE "file") == 0); if (print) fputs ("skipping test: symlinks not supported on this file system\n", stderr); return 77; } ASSERT (symlink (BASE "file", BASE "link2") == 0); ASSERT (symlink (BASE "nosuch", BASE "link3") == 0); ASSERT (symlink (BASE "link4", BASE "link4") == 0); ASSERT (func (BASE "link1", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); ASSERT (func (BASE "link1/", &st1) == 0); ASSERT (stat (BASE "link1", &st2) == 0); ASSERT (S_ISDIR (st1.st_mode)); ASSERT (S_ISDIR (st2.st_mode)); ASSERT (SAME_INODE (st1, st2)); ASSERT (func (BASE "link2", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); errno = 0; ASSERT (func (BASE "link2/", &st1) == -1); ASSERT (errno == ENOTDIR); ASSERT (func (BASE "link3", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); errno = 0; ASSERT (func (BASE "link3/", &st1) == -1); ASSERT (errno == ENOENT); ASSERT (func (BASE "link4", &st1) == 0); ASSERT (S_ISLNK (st1.st_mode)); errno = 0; ASSERT (func (BASE "link4/", &st1) == -1); ASSERT (errno == ELOOP); /* Cleanup. */ ASSERT (unlink (BASE "file") == 0); ASSERT (unlink (BASE "link1") == 0); ASSERT (unlink (BASE "link2") == 0); ASSERT (unlink (BASE "link3") == 0); ASSERT (unlink (BASE "link4") == 0); return 0; } gnuastro-0.5/bootstrapped/tests/localtime-buffer.h0000644000175000017500000000200313217200023017363 00000000000000/* Provide access to the last buffer returned by localtime() or gmtime(). Copyright (C) 2001-2003, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* written by Jim Meyering */ #include #if GETTIMEOFDAY_CLOBBERS_LOCALTIME || TZSET_CLOBBERS_LOCALTIME /* The address of the last buffer returned by localtime() or gmtime(). */ extern struct tm *localtime_buffer_addr; #endif gnuastro-0.5/bootstrapped/tests/localename.h0000644000175000017500000001103013217200023016243 00000000000000/* Determine name of the currently selected locale. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_LOCALENAME_H #define _GL_LOCALENAME_H #ifdef __cplusplus extern "C" { #endif /* Determine the current locale's name. It considers both the POSIX notion of locale name (see functions gl_locale_name_thread and gl_locale_name_posix) and the system notion of locale name (see function gl_locale_name_default). CATEGORY is a locale category abbreviation, as defined in , but not LC_ALL. E.g. LC_MESSAGES. CATEGORYNAME is the name of CATEGORY as a string, e.g. "LC_MESSAGES". Return the locale category's name, canonicalized into XPG syntax language[_territory][.codeset][@modifier] The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name (int category, const char *categoryname); /* Determine the current per-thread locale's name, as specified by uselocale() calls. CATEGORY is a locale category abbreviation, as defined in , but not LC_ALL. E.g. LC_MESSAGES. CATEGORYNAME is the name of CATEGORY as a string, e.g. "LC_MESSAGES". Return the locale category's name, canonicalized into XPG syntax language[_territory][.codeset][@modifier] or NULL if no locale has been specified for the current thread. The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_thread (int category, const char *categoryname); /* Determine the thread-independent current locale's name, as specified by setlocale() calls or by environment variables. CATEGORY is a locale category abbreviation, as defined in , but not LC_ALL. E.g. LC_MESSAGES. CATEGORYNAME is the name of CATEGORY as a string, e.g. "LC_MESSAGES". Return the locale category's name, canonicalized into XPG syntax language[_territory][.codeset][@modifier] or NULL if no locale has been specified to setlocale() or by environment variables. The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_posix (int category, const char *categoryname); /* Determine the default locale's name, as specified by environment variables. Return the locale category's name, or NULL if no locale has been specified by environment variables. The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_environ (int category, const char *categoryname); /* Determine the default locale's name. This is the current locale's name, if not specified by uselocale() calls, by setlocale() calls, or by environment variables. This locale name is usually determined by systems settings that the user can manipulate through a GUI. Quoting POSIX:2001: "All implementations shall define a locale as the default locale, to be invoked when no environment variables are set, or set to the empty string. This default locale can be the C locale or any other implementation-defined locale. Some implementations may provide facilities for local installation administrators to set the default locale, customizing it for each location. IEEE Std 1003.1-2001 does not require such a facility." The result must not be freed; it is statically allocated. */ extern const char * gl_locale_name_default (void) #if !(HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE \ || defined _WIN32 || defined __WIN32__ || defined __CYGWIN__) _GL_ATTRIBUTE_CONST #endif ; #ifdef __cplusplus } #endif #endif /* _GL_LOCALENAME_H */ gnuastro-0.5/bootstrapped/tests/test-isnanl.h0000644000175000017500000001077713217200024016426 00000000000000/* Test of isnanl() substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "minus-zero.h" #include "infinity.h" #include "nan.h" #include "macros.h" int main () { #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { unsigned int word[NWORDS]; long double value; } memory_long_double; /* Finite values. */ ASSERT (!isnanl (3.141L)); ASSERT (!isnanl (3.141e30L)); ASSERT (!isnanl (3.141e-30L)); ASSERT (!isnanl (-2.718L)); ASSERT (!isnanl (-2.718e30L)); ASSERT (!isnanl (-2.718e-30L)); ASSERT (!isnanl (0.0L)); ASSERT (!isnanl (minus_zerol)); /* Infinite values. */ ASSERT (!isnanl (Infinityl ())); ASSERT (!isnanl (- Infinityl ())); /* Quiet NaN. */ ASSERT (isnanl (NaNl ())); #if defined LDBL_EXPBIT0_WORD && defined LDBL_EXPBIT0_BIT /* A bit pattern that is different from a Quiet NaN. With a bit of luck, it's a Signalling NaN. */ { #if defined __powerpc__ && LDBL_MANT_DIG == 106 /* This is PowerPC "double double", a pair of two doubles. Inf and Nan are represented as the corresponding 64-bit IEEE values in the first double; the second is ignored. Manipulate only the first double. */ #undef NWORDS #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) #endif memory_long_double m; m.value = NaNl (); # if LDBL_EXPBIT0_BIT > 0 m.word[LDBL_EXPBIT0_WORD] ^= (unsigned int) 1 << (LDBL_EXPBIT0_BIT - 1); # else m.word[LDBL_EXPBIT0_WORD + (LDBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); # endif m.word[LDBL_EXPBIT0_WORD + (LDBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] |= (unsigned int) 1 << LDBL_EXPBIT0_BIT; ASSERT (isnanl (m.value)); } #endif #if ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Representation of an 80-bit 'long double' as an initializer for a sequence of 'unsigned int' words. */ # ifdef WORDS_BIGENDIAN # define LDBL80_WORDS(exponent,manthi,mantlo) \ { ((unsigned int) (exponent) << 16) | ((unsigned int) (manthi) >> 16), \ ((unsigned int) (manthi) << 16) | ((unsigned int) (mantlo) >> 16), \ (unsigned int) (mantlo) << 16 \ } # else # define LDBL80_WORDS(exponent,manthi,mantlo) \ { mantlo, manthi, exponent } # endif { /* Quiet NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0xC3333333, 0x00000000) }; ASSERT (isnanl (x.value)); } { /* Signalling NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x83333333, 0x00000000) }; ASSERT (isnanl (x.value)); } /* isnanl should return something for noncanonical values. */ { /* Pseudo-NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x40000001, 0x00000000) }; ASSERT (isnanl (x.value) || !isnanl (x.value)); } { /* Pseudo-Infinity. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x00000000, 0x00000000) }; ASSERT (isnanl (x.value) || !isnanl (x.value)); } { /* Pseudo-Zero. */ static memory_long_double x = { LDBL80_WORDS (0x4004, 0x00000000, 0x00000000) }; ASSERT (isnanl (x.value) || !isnanl (x.value)); } { /* Unnormalized number. */ static memory_long_double x = { LDBL80_WORDS (0x4000, 0x63333333, 0x00000000) }; ASSERT (isnanl (x.value) || !isnanl (x.value)); } { /* Pseudo-Denormal. */ static memory_long_double x = { LDBL80_WORDS (0x0000, 0x83333333, 0x00000000) }; ASSERT (isnanl (x.value) || !isnanl (x.value)); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/isnanl-nolibm.h0000644000175000017500000000231013217200023016706 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if HAVE_ISNANL_IN_LIBC /* Get declaration of isnan macro or (older) isnanl function. */ # include # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) # elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) # endif #else /* Test whether X is a NaN. */ # undef isnanl # define isnanl rpl_isnanl extern int isnanl (long double x); #endif gnuastro-0.5/bootstrapped/tests/test-isnanf.h0000644000175000017500000000410113217200024016400 00000000000000/* Test of isnanf() substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "minus-zero.h" #include "infinity.h" #include "nan.h" #include "macros.h" int main () { /* Finite values. */ ASSERT (!isnanf (3.141f)); ASSERT (!isnanf (3.141e30f)); ASSERT (!isnanf (3.141e-30f)); ASSERT (!isnanf (-2.718f)); ASSERT (!isnanf (-2.718e30f)); ASSERT (!isnanf (-2.718e-30f)); ASSERT (!isnanf (0.0f)); ASSERT (!isnanf (minus_zerof)); /* Infinite values. */ ASSERT (!isnanf (Infinityf ())); ASSERT (!isnanf (- Infinityf ())); /* Quiet NaN. */ ASSERT (isnanf (NaNf ())); #if defined FLT_EXPBIT0_WORD && defined FLT_EXPBIT0_BIT /* Signalling NaN. */ { #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; memory_float m; m.value = NaNf (); # if FLT_EXPBIT0_BIT > 0 m.word[FLT_EXPBIT0_WORD] ^= (unsigned int) 1 << (FLT_EXPBIT0_BIT - 1); # else m.word[FLT_EXPBIT0_WORD + (FLT_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); # endif if (FLT_EXPBIT0_WORD < NWORDS / 2) m.word[FLT_EXPBIT0_WORD + 1] |= (unsigned int) 1 << FLT_EXPBIT0_BIT; else m.word[0] |= (unsigned int) 1; ASSERT (isnanf (m.value)); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/isnanf-nolibm.h0000644000175000017500000000270213217200023016705 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if HAVE_ISNANF_IN_LIBC /* Get declaration of isnan macro or (older) isnanf function. */ # include # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) # elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) # else /* Get declaration of isnanf(), if not declared in . */ # if defined __sgi /* We can't include , because it conflicts with our definition of isnand. Therefore declare isnanf separately. */ extern int isnanf (float x); # endif # endif #else /* Test whether X is a NaN. */ # undef isnanf # define isnanf rpl_isnanf extern int isnanf (float x); #endif gnuastro-0.5/bootstrapped/tests/nan.h0000644000175000017500000000506313217200023014730 00000000000000/* Macros for not-a-number. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* IBM z/OS supports both hexadecimal and IEEE floating-point formats. The former does not support NaN and its isnan() implementation returns zero for all values. */ #if defined __MVS__ && defined __IBMC__ && !defined __BFP__ # error "NaN is not supported with IBM's hexadecimal floating-point format; please re-compile with -qfloat=ieee" #endif /* NaNf () returns a 'float' not-a-number. */ /* The Compaq (ex-DEC) C 6.4 compiler and the Microsoft MSVC 9 compiler choke on the expression 0.0 / 0.0. The IBM XL C compiler on z/OS complains. PGI 16.10 complains. */ #if (defined __DECC || defined _MSC_VER \ || (defined __MVS__ && defined __IBMC__) \ || defined __PGI) static float NaNf () { static float zero = 0.0f; return zero / zero; } #else # define NaNf() (0.0f / 0.0f) #endif /* NaNd () returns a 'double' not-a-number. */ /* The Compaq (ex-DEC) C 6.4 compiler and the Microsoft MSVC 9 compiler choke on the expression 0.0 / 0.0. The IBM XL C compiler on z/OS complains. PGI 16.10 complains. */ #if (defined __DECC || defined _MSC_VER \ || (defined __MVS__ && defined __IBMC__) \ || defined __PGI) static double NaNd () { static double zero = 0.0; return zero / zero; } #else # define NaNd() (0.0 / 0.0) #endif /* NaNl () returns a 'long double' not-a-number. */ /* On Irix 6.5, gcc 3.4.3 can't compute compile-time NaN, and needs the runtime type conversion. The Microsoft MSVC 9 compiler chokes on the expression 0.0L / 0.0L. The IBM XL C compiler on z/OS complains. PGI 16.10 complains. */ #ifdef __sgi static long double NaNl () { double zero = 0.0; return zero / zero; } #elif defined _MSC_VER || (defined __MVS__ && defined __IBMC__) || defined __PGI static long double NaNl () { static long double zero = 0.0L; return zero / zero; } #else # define NaNl() (0.0L / 0.0L) #endif gnuastro-0.5/bootstrapped/tests/infinity.h0000644000175000017500000000363713217200022016011 00000000000000/* Macros for infinity. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Infinityf () returns a 'float' +Infinity. */ /* The Microsoft MSVC 9 compiler chokes on the expression 1.0f / 0.0f. The IBM XL C compiler on z/OS complains. PGI 16.10 complains. */ #if defined _MSC_VER || (defined __MVS__ && defined __IBMC__) || defined __PGI static float Infinityf () { static float zero = 0.0f; return 1.0f / zero; } #else # define Infinityf() (1.0f / 0.0f) #endif /* Infinityd () returns a 'double' +Infinity. */ /* The Microsoft MSVC 9 compiler chokes on the expression 1.0 / 0.0. The IBM XL C compiler on z/OS complains. PGI 16.10 complains. */ #if defined _MSC_VER || (defined __MVS__ && defined __IBMC__) || defined __PGI static double Infinityd () { static double zero = 0.0; return 1.0 / zero; } #else # define Infinityd() (1.0 / 0.0) #endif /* Infinityl () returns a 'long double' +Infinity. */ /* The Microsoft MSVC 9 compiler chokes on the expression 1.0L / 0.0L. The IBM XL C compiler on z/OS complains. PGI 16.10 complains. */ #if defined _MSC_VER || (defined __MVS__ && defined __IBMC__) || defined __PGI static long double Infinityl () { static long double zero = 0.0L; return 1.0L / zero; } #else # define Infinityl() (1.0L / 0.0L) #endif gnuastro-0.5/bootstrapped/tests/minus-zero.h0000644000175000017500000000452613217200023016267 00000000000000/* Macros for floating-point negative zero. Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Keep in sync with m4/minus-zero.m4! */ #include /* minus_zerof represents the value -0.0f. */ /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0f. ICC 10.0 has a bug when optimizing the expression -zero. The expression -FLT_MIN * FLT_MIN does not work when cross-compiling to PowerPC on Mac OS X 10.5. */ #if defined __hpux || defined __sgi || defined __ICC static float compute_minus_zerof (void) { return -FLT_MIN * FLT_MIN; } # define minus_zerof compute_minus_zerof () #else float minus_zerof = -0.0f; #endif /* minus_zerod represents the value -0.0. */ /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0. ICC 10.0 has a bug when optimizing the expression -zero. The expression -DBL_MIN * DBL_MIN does not work when cross-compiling to PowerPC on Mac OS X 10.5. */ #if defined __hpux || defined __sgi || defined __ICC static double compute_minus_zerod (void) { return -DBL_MIN * DBL_MIN; } # define minus_zerod compute_minus_zerod () #else double minus_zerod = -0.0; #endif /* minus_zerol represents the value -0.0L. */ /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0L. IRIX cc can't put -0.0L into .data, but can compute at runtime. ICC 10.0 has a bug when optimizing the expression -zero. The expression -LDBL_MIN * LDBL_MIN does not work when cross-compiling to PowerPC on Mac OS X 10.5. */ #if defined __hpux || defined __sgi || defined __ICC static long double compute_minus_zerol (void) { return -LDBL_MIN * LDBL_MIN; } # define minus_zerol compute_minus_zerol () #else long double minus_zerol = -0.0L; #endif gnuastro-0.5/bootstrapped/tests/test-isnand.h0000644000175000017500000000402513217200024016403 00000000000000/* Test of isnand() substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "minus-zero.h" #include "infinity.h" #include "nan.h" #include "macros.h" int main () { /* Finite values. */ ASSERT (!isnand (3.141)); ASSERT (!isnand (3.141e30)); ASSERT (!isnand (3.141e-30)); ASSERT (!isnand (-2.718)); ASSERT (!isnand (-2.718e30)); ASSERT (!isnand (-2.718e-30)); ASSERT (!isnand (0.0)); ASSERT (!isnand (minus_zerod)); /* Infinite values. */ ASSERT (!isnand (Infinityd ())); ASSERT (!isnand (- Infinityd ())); /* Quiet NaN. */ ASSERT (isnand (NaNd ())); #if defined DBL_EXPBIT0_WORD && defined DBL_EXPBIT0_BIT /* Signalling NaN. */ { #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; memory_double m; m.value = NaNd (); # if DBL_EXPBIT0_BIT > 0 m.word[DBL_EXPBIT0_WORD] ^= (unsigned int) 1 << (DBL_EXPBIT0_BIT - 1); # else m.word[DBL_EXPBIT0_WORD + (DBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); # endif m.word[DBL_EXPBIT0_WORD + (DBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] |= (unsigned int) 1 << DBL_EXPBIT0_BIT; ASSERT (isnand (m.value)); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/isnand-nolibm.h0000644000175000017500000000221713217200023016704 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if HAVE_ISNAND_IN_LIBC /* Get declaration of isnan macro. */ # include # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnand # define isnand(x) __builtin_isnan ((double)(x)) # else # undef isnand # define isnand(x) isnan ((double)(x)) # endif #else /* Test whether X is a NaN. */ # undef isnand # define isnand rpl_isnand extern int isnand (double x); #endif gnuastro-0.5/bootstrapped/tests/float+.h0000644000175000017500000001274613217200022015341 00000000000000/* Supplemental information about the floating-point formats. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _FLOATPLUS_H #define _FLOATPLUS_H #include #include /* Number of bits in the mantissa of a floating-point number, including the "hidden bit". */ #if FLT_RADIX == 2 # define FLT_MANT_BIT FLT_MANT_DIG # define DBL_MANT_BIT DBL_MANT_DIG # define LDBL_MANT_BIT LDBL_MANT_DIG #elif FLT_RADIX == 4 # define FLT_MANT_BIT (FLT_MANT_DIG * 2) # define DBL_MANT_BIT (DBL_MANT_DIG * 2) # define LDBL_MANT_BIT (LDBL_MANT_DIG * 2) #elif FLT_RADIX == 16 # define FLT_MANT_BIT (FLT_MANT_DIG * 4) # define DBL_MANT_BIT (DBL_MANT_DIG * 4) # define LDBL_MANT_BIT (LDBL_MANT_DIG * 4) #endif /* Bit mask that can be used to mask the exponent, as an unsigned number. */ #define FLT_EXP_MASK ((FLT_MAX_EXP - FLT_MIN_EXP) | 7) #define DBL_EXP_MASK ((DBL_MAX_EXP - DBL_MIN_EXP) | 7) #define LDBL_EXP_MASK ((LDBL_MAX_EXP - LDBL_MIN_EXP) | 7) /* Number of bits used for the exponent of a floating-point number, including the exponent's sign. */ #define FLT_EXP_BIT \ (FLT_EXP_MASK < 0x100 ? 8 : \ FLT_EXP_MASK < 0x200 ? 9 : \ FLT_EXP_MASK < 0x400 ? 10 : \ FLT_EXP_MASK < 0x800 ? 11 : \ FLT_EXP_MASK < 0x1000 ? 12 : \ FLT_EXP_MASK < 0x2000 ? 13 : \ FLT_EXP_MASK < 0x4000 ? 14 : \ FLT_EXP_MASK < 0x8000 ? 15 : \ FLT_EXP_MASK < 0x10000 ? 16 : \ FLT_EXP_MASK < 0x20000 ? 17 : \ FLT_EXP_MASK < 0x40000 ? 18 : \ FLT_EXP_MASK < 0x80000 ? 19 : \ FLT_EXP_MASK < 0x100000 ? 20 : \ FLT_EXP_MASK < 0x200000 ? 21 : \ FLT_EXP_MASK < 0x400000 ? 22 : \ FLT_EXP_MASK < 0x800000 ? 23 : \ FLT_EXP_MASK < 0x1000000 ? 24 : \ FLT_EXP_MASK < 0x2000000 ? 25 : \ FLT_EXP_MASK < 0x4000000 ? 26 : \ FLT_EXP_MASK < 0x8000000 ? 27 : \ FLT_EXP_MASK < 0x10000000 ? 28 : \ FLT_EXP_MASK < 0x20000000 ? 29 : \ FLT_EXP_MASK < 0x40000000 ? 30 : \ FLT_EXP_MASK <= 0x7fffffff ? 31 : \ 32) #define DBL_EXP_BIT \ (DBL_EXP_MASK < 0x100 ? 8 : \ DBL_EXP_MASK < 0x200 ? 9 : \ DBL_EXP_MASK < 0x400 ? 10 : \ DBL_EXP_MASK < 0x800 ? 11 : \ DBL_EXP_MASK < 0x1000 ? 12 : \ DBL_EXP_MASK < 0x2000 ? 13 : \ DBL_EXP_MASK < 0x4000 ? 14 : \ DBL_EXP_MASK < 0x8000 ? 15 : \ DBL_EXP_MASK < 0x10000 ? 16 : \ DBL_EXP_MASK < 0x20000 ? 17 : \ DBL_EXP_MASK < 0x40000 ? 18 : \ DBL_EXP_MASK < 0x80000 ? 19 : \ DBL_EXP_MASK < 0x100000 ? 20 : \ DBL_EXP_MASK < 0x200000 ? 21 : \ DBL_EXP_MASK < 0x400000 ? 22 : \ DBL_EXP_MASK < 0x800000 ? 23 : \ DBL_EXP_MASK < 0x1000000 ? 24 : \ DBL_EXP_MASK < 0x2000000 ? 25 : \ DBL_EXP_MASK < 0x4000000 ? 26 : \ DBL_EXP_MASK < 0x8000000 ? 27 : \ DBL_EXP_MASK < 0x10000000 ? 28 : \ DBL_EXP_MASK < 0x20000000 ? 29 : \ DBL_EXP_MASK < 0x40000000 ? 30 : \ DBL_EXP_MASK <= 0x7fffffff ? 31 : \ 32) #define LDBL_EXP_BIT \ (LDBL_EXP_MASK < 0x100 ? 8 : \ LDBL_EXP_MASK < 0x200 ? 9 : \ LDBL_EXP_MASK < 0x400 ? 10 : \ LDBL_EXP_MASK < 0x800 ? 11 : \ LDBL_EXP_MASK < 0x1000 ? 12 : \ LDBL_EXP_MASK < 0x2000 ? 13 : \ LDBL_EXP_MASK < 0x4000 ? 14 : \ LDBL_EXP_MASK < 0x8000 ? 15 : \ LDBL_EXP_MASK < 0x10000 ? 16 : \ LDBL_EXP_MASK < 0x20000 ? 17 : \ LDBL_EXP_MASK < 0x40000 ? 18 : \ LDBL_EXP_MASK < 0x80000 ? 19 : \ LDBL_EXP_MASK < 0x100000 ? 20 : \ LDBL_EXP_MASK < 0x200000 ? 21 : \ LDBL_EXP_MASK < 0x400000 ? 22 : \ LDBL_EXP_MASK < 0x800000 ? 23 : \ LDBL_EXP_MASK < 0x1000000 ? 24 : \ LDBL_EXP_MASK < 0x2000000 ? 25 : \ LDBL_EXP_MASK < 0x4000000 ? 26 : \ LDBL_EXP_MASK < 0x8000000 ? 27 : \ LDBL_EXP_MASK < 0x10000000 ? 28 : \ LDBL_EXP_MASK < 0x20000000 ? 29 : \ LDBL_EXP_MASK < 0x40000000 ? 30 : \ LDBL_EXP_MASK <= 0x7fffffff ? 31 : \ 32) /* Number of bits used for a floating-point number: the mantissa (not counting the "hidden bit", since it may or may not be explicit), the exponent, and the sign. */ #define FLT_TOTAL_BIT ((FLT_MANT_BIT - 1) + FLT_EXP_BIT + 1) #define DBL_TOTAL_BIT ((DBL_MANT_BIT - 1) + DBL_EXP_BIT + 1) #define LDBL_TOTAL_BIT ((LDBL_MANT_BIT - 1) + LDBL_EXP_BIT + 1) /* Number of bytes used for a floating-point number. This can be smaller than the 'sizeof'. For example, on i386 systems, 'long double' most often have LDBL_MANT_BIT = 64, LDBL_EXP_BIT = 16, hence LDBL_TOTAL_BIT = 80 bits, i.e. 10 bytes of consecutive memory, but sizeof (long double) = 12 or = 16. */ #define SIZEOF_FLT ((FLT_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) #define SIZEOF_DBL ((DBL_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) #define SIZEOF_LDBL ((LDBL_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) /* Verify that SIZEOF_FLT <= sizeof (float) etc. */ typedef int verify_sizeof_flt[SIZEOF_FLT <= sizeof (float) ? 1 : -1]; typedef int verify_sizeof_dbl[SIZEOF_DBL <= sizeof (double) ? 1 : - 1]; typedef int verify_sizeof_ldbl[SIZEOF_LDBL <= sizeof (long double) ? 1 : - 1]; #endif /* _FLOATPLUS_H */ gnuastro-0.5/bootstrapped/tests/ignore-value.h0000644000175000017500000000423513217200022016550 00000000000000/* ignore a function return without a compiler warning. -*- coding: utf-8 -*- Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Jim Meyering, Eric Blake and Pádraig Brady. */ /* Use "ignore_value" to avoid a warning when using a function declared with gcc's warn_unused_result attribute, but for which you really do want to ignore the result. Traditionally, people have used a "(void)" cast to indicate that a function's return value is deliberately unused. However, if the function is declared with __attribute__((warn_unused_result)), gcc issues a warning even with the cast. Caution: most of the time, you really should heed gcc's warning, and check the return value. However, in those exceptional cases in which you're sure you know what you're doing, use this function. For the record, here's one of the ignorable warnings: "copy.c:233: warning: ignoring return value of 'fchown', declared with attribute warn_unused_result". */ #ifndef _GL_IGNORE_VALUE_H #define _GL_IGNORE_VALUE_H /* Normally casting an expression to void discards its value, but GCC versions 3.4 and newer have __attribute__ ((__warn_unused_result__)) which may cause unwanted diagnostics in that case. Use __typeof__ and __extension__ to work around the problem, if the workaround is known to be needed. */ #if 3 < __GNUC__ + (4 <= __GNUC_MINOR__) # define ignore_value(x) \ (__extension__ ({ __typeof__ (x) __x = (x); (void) __x; })) #else # define ignore_value(x) ((void) (x)) #endif #endif gnuastro-0.5/bootstrapped/tests/test-getopt_long.h0000644000175000017500000017550613217200023017464 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ static int a_seen; static int b_seen; static int q_seen; static const struct option long_options_required[] = { { "alpha", no_argument, NULL, 'a' }, { "beta", no_argument, &b_seen, 1 }, { "prune", required_argument, NULL, 'p' }, { "quetsche", required_argument, &q_seen, 1 }, { "xtremely-",no_argument, NULL, 1003 }, { "xtra", no_argument, NULL, 1001 }, { "xtreme", no_argument, NULL, 1002 }, { "xtremely", no_argument, NULL, 1003 }, { NULL, 0, NULL, 0 } }; static const struct option long_options_optional[] = { { "alpha", no_argument, NULL, 'a' }, { "beta", no_argument, &b_seen, 1 }, { "prune", optional_argument, NULL, 'p' }, { "quetsche", optional_argument, &q_seen, 1 }, { NULL, 0, NULL, 0 } }; static void getopt_long_loop (int argc, const char **argv, const char *options, const struct option *long_options, const char **p_value, const char **q_value, int *non_options_count, const char **non_options, int *unrecognized) { int option_index = -1; int c; opterr = 0; q_seen = 0; while ((c = getopt_long (argc, (char **) argv, options, long_options, &option_index)) != -1) { switch (c) { case 0: /* An option with a non-NULL flag pointer was processed. */ if (q_seen) *q_value = optarg; break; case 'a': a_seen++; break; case 'b': b_seen = 1; break; case 'p': *p_value = optarg; break; case 'q': *q_value = optarg; break; case '\1': /* Must only happen with option '-' at the beginning. */ ASSERT (options[0] == '-'); non_options[(*non_options_count)++] = optarg; break; case ':': /* Must only happen with option ':' at the beginning. */ ASSERT (options[0] == ':' || ((options[0] == '-' || options[0] == '+') && options[1] == ':')); FALLTHROUGH; case '?': *unrecognized = optopt; break; default: *unrecognized = c; break; } } } /* Reduce casting, so we can use string literals elsewhere. getopt_long takes an array of char*, but luckily does not modify those elements, so we can pass const char*. */ static int do_getopt_long (int argc, const char **argv, const char *shortopts, const struct option *longopts, int *longind) { return getopt_long (argc, (char **) argv, shortopts, longopts, longind); } static void test_getopt_long (void) { int start; /* Test disambiguation of options. */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xt"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtr"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtra"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1001); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtre"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtrem"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtreme"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1002); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtremel"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1003); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--xtremely"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1003); } /* Check that -W handles unknown options. */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 'W'); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-Wunknown"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", long_options_required, &option_index); /* glibc and BSD behave differently here, but for now, we allow both behaviors since W support is not frequently used. */ if (c == '?') { ASSERT (optopt == 0); ASSERT (optarg == NULL); } else { ASSERT (c == 'W'); ASSERT (strcmp (optarg, "unknown") == 0); } } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "unknown"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", long_options_required, &option_index); /* glibc and BSD behave differently here, but for now, we allow both behaviors since W support is not frequently used. */ if (c == '?') { ASSERT (optopt == 0); ASSERT (optarg == NULL); } else { ASSERT (c == 'W'); ASSERT (strcmp (optarg, "unknown") == 0); } } /* Test that 'W' does not dump core: https://sourceware.org/bugzilla/show_bug.cgi?id=12922 */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "dummy"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long (argc, argv, "W;", NULL, &option_index); ASSERT (c == 'W'); ASSERT (optind == 2); } /* Test processing of boolean short options. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ba"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } /* Test processing of boolean long options. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--alpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--beta"; argv[argc++] = "--alpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--alpha"; argv[argc++] = "--beta"; argv[argc++] = "--alpha"; argv[argc++] = "--beta"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of boolean long options via -W. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Walpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abW;", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "beta"; argv[argc++] = "-W"; argv[argc++] = "alpha"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "aW;b", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Walpha"; argv[argc++] = "-Wbeta"; argv[argc++] = "-Walpha"; argv[argc++] = "-Wbeta"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of short options with arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-q"; argv[argc++] = "baz"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of long options with arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "--q"; argv[argc++] = "baz"; argv[argc++] = "--p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Test processing of long options with arguments via -W. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:q:W;", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p:W;q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-Wq"; argv[argc++] = "baz"; argv[argc++] = "-W"; argv[argc++] = "p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 6); } /* Test processing of short options with optional arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } /* Test processing of long options with optional arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p="; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && *p_value == '\0'); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "--p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } /* Test processing of long options with optional arguments via -W. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp=foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::W;", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::q::W;", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-Wp="; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && *p_value == '\0'); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "p="; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;p::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && *p_value == '\0'); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "W;abp::q::", long_options_optional, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); /* ASSERT (p_value == NULL); */ ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } /* Check that invalid options are recognized. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); } /* Check that unexpected arguments are recognized. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "--a="; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'a'); ASSERT (optind == 4); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "--b="; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); /* When flag is non-zero, glibc sets optopt anyway, but BSD leaves optopt unchanged. */ ASSERT (unrecognized == 1 || unrecognized == 0); ASSERT (optind == 4); } /* Check that by default, non-options arguments are moved to the end. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } /* Check that '--' ends the argument processing. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[20]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "--") == 0); ASSERT (strcmp (argv[5], "donald") == 0); ASSERT (strcmp (argv[6], "duck") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); } /* Check that the '-' flag causes non-options to be returned in order. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "-abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 3); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); } /* Check that '--' ends the argument processing. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[20]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "-abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); if (non_options_count == 2) { /* glibc behaviour. */ ASSERT (non_options_count == 2); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); } else { /* Another valid behaviour. */ ASSERT (non_options_count == 7); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "-b") == 0); ASSERT (strcmp (non_options[3], "foo") == 0); ASSERT (strcmp (non_options[4], "-q") == 0); ASSERT (strcmp (non_options[5], "johnny") == 0); ASSERT (strcmp (non_options[6], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 12); } } /* Check that the '-' flag has to come first. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:-", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } /* Check that the '+' flag causes the first non-option to terminate the loop. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "+abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); } for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-+"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "+abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == '+'); ASSERT (optind == 2); } /* Check that '--' ends the argument processing. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[20]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "+abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); } /* Check that the '+' flag has to come first. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:+", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } } /* Test behavior of getopt_long when POSIXLY_CORRECT is set in the environment. Options with optional arguments should not change behavior just because of an environment variable. https://lists.gnu.org/r/bug-m4/2006-09/msg00028.html */ static void test_getopt_long_posix (void) { int start; /* Check that POSIXLY_CORRECT stops parsing the same as leading '+'. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "abp:q:", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); } /* Check that POSIXLY_CORRECT doesn't change optional arguments. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "p::", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); } /* Check that leading - still sees options after non-options. */ for (start = 0; start <= 1; start++) { const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; int argc = 0; const char *argv[10]; a_seen = 0; b_seen = 0; argv[argc++] = "program"; argv[argc++] = "-a"; argv[argc++] = "billy"; argv[argc++] = "-b"; argv[argc] = NULL; optind = start; getopt_long_loop (argc, argv, "-ab", long_options_required, &p_value, &q_value, &non_options_count, non_options, &unrecognized); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 1); ASSERT (strcmp (non_options[0], "billy") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); } } /* Reduce casting, so we can use string literals elsewhere. getopt_long_only takes an array of char*, but luckily does not modify those elements, so we can pass const char*. */ static int do_getopt_long_only (int argc, const char **argv, const char *shortopts, const struct option *longopts, int *longind) { return getopt_long_only (argc, (char **) argv, shortopts, longopts, longind); } static void test_getopt_long_only (void) { /* Test disambiguation of options. */ { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == 'x'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--x"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc] = NULL; optind = 1; opterr = 0; b_seen = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == 'b'); ASSERT (b_seen == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "--b"; argv[argc] = NULL; optind = 1; opterr = 0; b_seen = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == 0); ASSERT (b_seen == 1); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xt"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xt"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx", long_options_required, &option_index); ASSERT (c == '?'); ASSERT (optopt == 0); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtra"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); ASSERT (c == 1001); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtreme"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx:", long_options_required, &option_index); ASSERT (c == 1002); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtremel"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "ab", long_options_required, &option_index); /* glibc getopt_long_only is intentionally different from getopt_long when handling a prefix that is common to two spellings, when both spellings have the same option directives. BSD getopt_long_only treats both cases the same. */ ASSERT (c == 1003 || c == '?'); ASSERT (optind == 2); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtremel"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx::", long_options_required, &option_index); /* glibc getopt_long_only is intentionally different from getopt_long when handling a prefix that is common to two spellings, when both spellings have the same option directives. BSD getopt_long_only treats both cases the same. */ ASSERT (c == 1003 || c == '?'); ASSERT (optind == 2); ASSERT (optarg == NULL); } { int argc = 0; const char *argv[10]; int option_index; int c; argv[argc++] = "program"; argv[argc++] = "-xtras"; argv[argc] = NULL; optind = 1; opterr = 0; c = do_getopt_long_only (argc, argv, "abx::", long_options_required, &option_index); ASSERT (c == 'x'); ASSERT (strcmp (optarg, "tras") == 0); } } gnuastro-0.5/bootstrapped/tests/test-getopt.h0000644000175000017500000012565513217200023016445 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* The glibc/gnulib implementation of getopt supports setting optind = 0, but not all other implementations do. This matters for getopt. But for getopt_long, we require GNU compatibility. */ #if defined __GETOPT_PREFIX || (__GLIBC__ >= 2 && !defined __UCLIBC__) # define OPTIND_MIN 0 #elif HAVE_DECL_OPTRESET # define OPTIND_MIN (optreset = 1) #else # define OPTIND_MIN 1 #endif static void getopt_loop (int argc, const char **argv, const char *options, int *a_seen, int *b_seen, const char **p_value, const char **q_value, int *non_options_count, const char **non_options, int *unrecognized, bool *message_issued) { int c; int pos = ftell (stderr); while ((c = getopt (argc, (char **) argv, options)) != -1) { switch (c) { case 'a': (*a_seen)++; break; case 'b': (*b_seen)++; break; case 'p': *p_value = optarg; break; case 'q': *q_value = optarg; break; case '\1': /* Must only happen with option '-' at the beginning. */ ASSERT (options[0] == '-'); non_options[(*non_options_count)++] = optarg; break; case ':': /* Must only happen with option ':' at the beginning. */ ASSERT (options[0] == ':' || ((options[0] == '-' || options[0] == '+') && options[1] == ':')); FALLTHROUGH; case '?': *unrecognized = optopt; break; default: *unrecognized = c; break; } } *message_issued = pos < ftell (stderr); } static void test_getopt (void) { int start; bool posixly = !!getenv ("POSIXLY_CORRECT"); /* See comment in getopt.c: glibc gets a LSB-compliant getopt. Standalone applications get a POSIX-compliant getopt. */ #if defined __GETOPT_PREFIX || !(__GLIBC__ >= 2 || defined __MINGW32__) /* Using getopt from gnulib or from a non-glibc system. */ posixly = true; #endif /* Test processing of boolean options. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ba"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-a"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "ab", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 2); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } /* Test processing of options with arguments. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ab"; argv[argc++] = "-q"; argv[argc++] = "baz"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 1); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value != NULL && strcmp (q_value, "baz") == 0); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); ASSERT (!output); } #if GNULIB_TEST_GETOPT_GNU /* Test processing of options with optional arguments. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-pfoo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p::q::", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "p::q::", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp::q::", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 3); ASSERT (!output); } #endif /* GNULIB_TEST_GETOPT_GNU */ /* Check that invalid options are recognized; and that both opterr and leading ':' can silence output. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 42; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); ASSERT (output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 0; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-x"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, ":abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'x'); ASSERT (optind == 5); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 42; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); ASSERT (output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 0; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc++] = "foo"; argv[argc++] = "-:"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, ":abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "foo") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == ':'); ASSERT (optind == 5); ASSERT (!output); } /* Check for missing argument behavior. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ap"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ap"; argv[argc] = NULL; optind = start; opterr = 0; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-ap"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, ":abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (!output); } /* Check that by default, non-options arguments are moved to the end. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); ASSERT (!output); } } /* Check that '--' ends the argument processing. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[20]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "--") == 0); ASSERT (strcmp (argv[5], "donald") == 0); ASSERT (strcmp (argv[6], "duck") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 5); ASSERT (!output); } } #if GNULIB_TEST_GETOPT_GNU /* Check that the '-' flag causes non-options to be returned in order. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "-abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 3); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); ASSERT (!output); } /* Check that '--' ends the argument processing. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[20]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "-abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (!output); if (non_options_count == 2) { /* glibc behaviour. */ ASSERT (non_options_count == 2); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 7); } else { /* Another valid behaviour. */ ASSERT (non_options_count == 7); ASSERT (strcmp (non_options[0], "donald") == 0); ASSERT (strcmp (non_options[1], "duck") == 0); ASSERT (strcmp (non_options[2], "-b") == 0); ASSERT (strcmp (non_options[3], "foo") == 0); ASSERT (strcmp (non_options[4], "-q") == 0); ASSERT (strcmp (non_options[5], "johnny") == 0); ASSERT (strcmp (non_options[6], "bar") == 0); ASSERT (unrecognized == 0); ASSERT (optind == 12); } } /* Check that the '-' flag has to come first. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:-", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); ASSERT (!output); } } /* Check that the '+' flag causes the first non-option to terminate the loop. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "+abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-+"; argv[argc] = NULL; optind = start; getopt_loop (argc, argv, "+abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == '+'); ASSERT (optind == 2); ASSERT (output); } /* Check that '--' ends the argument processing. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[20]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "--"; argv[argc++] = "-b"; argv[argc++] = "foo"; argv[argc++] = "-q"; argv[argc++] = "johnny"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "+abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "--") == 0); ASSERT (strcmp (argv[7], "-b") == 0); ASSERT (strcmp (argv[8], "foo") == 0); ASSERT (strcmp (argv[9], "-q") == 0); ASSERT (strcmp (argv[10], "johnny") == 0); ASSERT (strcmp (argv[11], "bar") == 0); ASSERT (argv[12] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } #endif /* GNULIB_TEST_GETOPT_GNU */ /* Check that the '+' flag has to come first. */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "abp:q:+", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); if (posixly) { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } else { ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "-p") == 0); ASSERT (strcmp (argv[2], "billy") == 0); ASSERT (strcmp (argv[3], "-a") == 0); ASSERT (strcmp (argv[4], "donald") == 0); ASSERT (strcmp (argv[5], "duck") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 1); ASSERT (b_seen == 0); ASSERT (p_value != NULL && strcmp (p_value, "billy") == 0); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 4); ASSERT (!output); } } #if GNULIB_TEST_GETOPT_GNU /* If GNU extensions are supported, require compliance with POSIX interpretation on leading '+' behavior. http://austingroupbugs.net/view.php?id=191 */ for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "donald"; argv[argc++] = "-p"; argv[argc++] = "billy"; argv[argc++] = "duck"; argv[argc++] = "-a"; argv[argc++] = "bar"; argv[argc] = NULL; optind = start; opterr = 1; getopt_loop (argc, argv, "+:abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (strcmp (argv[0], "program") == 0); ASSERT (strcmp (argv[1], "donald") == 0); ASSERT (strcmp (argv[2], "-p") == 0); ASSERT (strcmp (argv[3], "billy") == 0); ASSERT (strcmp (argv[4], "duck") == 0); ASSERT (strcmp (argv[5], "-a") == 0); ASSERT (strcmp (argv[6], "bar") == 0); ASSERT (argv[7] == NULL); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 0); ASSERT (optind == 1); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-p"; argv[argc] = NULL; optind = start; getopt_loop (argc, argv, "+:abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 0); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 2); ASSERT (!output); } for (start = OPTIND_MIN; start <= 1; start++) { int a_seen = 0; int b_seen = 0; const char *p_value = NULL; const char *q_value = NULL; int non_options_count = 0; const char *non_options[10]; int unrecognized = 0; bool output; int argc = 0; const char *argv[10]; argv[argc++] = "program"; argv[argc++] = "-b"; argv[argc++] = "-p"; argv[argc] = NULL; optind = start; getopt_loop (argc, argv, "+:abp:q:", &a_seen, &b_seen, &p_value, &q_value, &non_options_count, non_options, &unrecognized, &output); ASSERT (a_seen == 0); ASSERT (b_seen == 1); ASSERT (p_value == NULL); ASSERT (q_value == NULL); ASSERT (non_options_count == 0); ASSERT (unrecognized == 'p'); ASSERT (optind == 3); ASSERT (!output); } /* Check that 'W' does not dump core: https://sourceware.org/bugzilla/show_bug.cgi?id=12922 Technically, POSIX says the presence of ';' in the opt-string gives unspecified behavior, so we only test this when GNU compliance is desired. */ for (start = OPTIND_MIN; start <= 1; start++) { int argc = 0; const char *argv[10]; int pos = ftell (stderr); argv[argc++] = "program"; argv[argc++] = "-W"; argv[argc++] = "dummy"; argv[argc] = NULL; optind = start; opterr = 1; ASSERT (getopt (argc, (char **) argv, "W;") == 'W'); ASSERT (ftell (stderr) == pos); ASSERT (optind == 2); } #endif /* GNULIB_TEST_GETOPT_GNU */ } gnuastro-0.5/bootstrapped/tests/test-getopt-main.h0000644000175000017500000000411413217200023017351 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include "signature.h" SIGNATURE_CHECK (getopt, int, (int, char * const[], char const *)); #include #include #include #include /* This test intentionally remaps stderr. So, we arrange to have fd 10 (outside the range of interesting fd's during the test) set up to duplicate the original stderr. */ #define BACKUP_STDERR_FILENO 10 #define ASSERT_STREAM myerr #include "macros.h" static FILE *myerr; #include "test-getopt.h" #if TEST_GETOPT_GNU # include "test-getopt_long.h" #endif int main (void) { /* This test validates that stderr is used correctly, so move the original into fd 10. */ if (dup2 (STDERR_FILENO, BACKUP_STDERR_FILENO) != BACKUP_STDERR_FILENO || (myerr = fdopen (BACKUP_STDERR_FILENO, "w")) == NULL) return 2; ASSERT (freopen (TEST_GETOPT_TMP_NAME, "w", stderr) == stderr); /* These default values are required by POSIX. */ ASSERT (optind == 1); ASSERT (opterr != 0); setenv ("POSIXLY_CORRECT", "1", 1); test_getopt (); #if TEST_GETOPT_GNU test_getopt_long_posix (); #endif unsetenv ("POSIXLY_CORRECT"); test_getopt (); #if TEST_GETOPT_GNU test_getopt_long (); test_getopt_long_only (); #endif ASSERT (fclose (stderr) == 0); ASSERT (remove (TEST_GETOPT_TMP_NAME) == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-ftruncate.sh0000755000175000017500000000010613217200023017303 00000000000000#!/bin/sh exec ./test-ftruncate${EXEEXT} "$srcdir/test-ftruncate.sh" gnuastro-0.5/bootstrapped/tests/stat-w32.h0000644000175000017500000000306113217200023015534 00000000000000/* Core of implementation of fstat and stat for native Windows. Copyright (C) 2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _STAT_W32_H #define _STAT_W32_H 1 /* Converts a FILETIME to GMT time since 1970-01-01 00:00:00. */ #if _GL_WINDOWS_STAT_TIMESPEC extern struct timespec _gl_convert_FILETIME_to_timespec (const FILETIME *ft); #else extern time_t _gl_convert_FILETIME_to_POSIX (const FILETIME *ft); #endif /* Fill *BUF with information about the file designated by H. PATH is the file name, if known, otherwise NULL. Return 0 if successful, or -1 with errno set upon failure. */ extern int _gl_fstat_by_handle (HANDLE h, const char *path, struct stat *buf); /* Bitmasks for st_mode. */ #define S_IREAD_UGO (_S_IREAD | (_S_IREAD >> 3) | (_S_IREAD >> 6)) #define S_IWRITE_UGO (_S_IWRITE | (_S_IWRITE >> 3) | (_S_IWRITE >> 6)) #define S_IEXEC_UGO (_S_IEXEC | (_S_IEXEC >> 3) | (_S_IEXEC >> 6)) #endif /* _STAT_W32_H */ gnuastro-0.5/bootstrapped/tests/fpucw.h0000644000175000017500000001120013217200022015265 00000000000000/* Manipulating the FPU control word. -*- coding: utf-8 -*- Copyright (C) 2007-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _FPUCW_H #define _FPUCW_H /* The i386 floating point hardware (the 387 compatible FPU, not the modern SSE/SSE2 hardware) has a controllable rounding precision. It is specified through the 'PC' bits in the FPU control word ('fctrl' register). (See the GNU libc i386 header for details.) On some platforms, such as Linux or Solaris, the default precision setting is set to "extended precision". This means that 'long double' instructions operate correctly, but 'double' computations often produce slightly different results as on strictly IEEE 754 conforming systems. On some platforms, such as NetBSD, the default precision is set to "double precision". This means that 'long double' instructions will operate only as 'double', i.e. lead to wrong results. Similarly on FreeBSD 6.4, at least for the division of 'long double' numbers. The FPU control word is under control of the application, i.e. it is not required to be set either way by the ABI. (In fact, the i386 ABI https://www.linux-mips.org/pub/linux/mips/doc/ABI/abi386-4.pdf page 3-12 = page 38 is not clear about it. But in any case, gcc treats the control word like a "preserved" register: it emits code that assumes that the control word is preserved across calls, and it restores the control word at the end of functions that modify it.) See Vincent Lefèvre's page https://www.vinc17.net/research/extended.en.html for a good explanation. See http://www.uwsg.iu.edu/hypermail/linux/kernel/0103.0/0453.html for some argumentation which setting should be the default. */ /* This header file provides the following facilities: fpucw_t integral type holding the value of 'fctrl' FPU_PC_MASK bit mask denoting the precision control FPU_PC_DOUBLE precision control for 53 bits mantissa FPU_PC_EXTENDED precision control for 64 bits mantissa GET_FPUCW () yields the current FPU control word SET_FPUCW (word) sets the FPU control word DECL_LONG_DOUBLE_ROUNDING variable declaration for BEGIN/END_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING () starts a sequence of instructions with 'long double' safe operation precision END_LONG_DOUBLE_ROUNDING () ends a sequence of instructions with 'long double' safe operation precision */ /* Inline assembler like this works only with GNU C. */ #if (defined __i386__ || defined __x86_64__) && defined __GNUC__ typedef unsigned short fpucw_t; /* glibc calls this fpu_control_t */ # define FPU_PC_MASK 0x0300 # define FPU_PC_DOUBLE 0x200 /* glibc calls this _FPU_DOUBLE */ # define FPU_PC_EXTENDED 0x300 /* glibc calls this _FPU_EXTENDED */ # define GET_FPUCW() \ ({ fpucw_t _cw; \ __asm__ __volatile__ ("fnstcw %0" : "=m" (*&_cw)); \ _cw; \ }) # define SET_FPUCW(word) \ (void)({ fpucw_t _ncw = (word); \ __asm__ __volatile__ ("fldcw %0" : : "m" (*&_ncw)); \ }) # define DECL_LONG_DOUBLE_ROUNDING \ fpucw_t oldcw; # define BEGIN_LONG_DOUBLE_ROUNDING() \ (void)(oldcw = GET_FPUCW (), \ SET_FPUCW ((oldcw & ~FPU_PC_MASK) | FPU_PC_EXTENDED)) # define END_LONG_DOUBLE_ROUNDING() \ SET_FPUCW (oldcw) #else typedef unsigned int fpucw_t; # define FPU_PC_MASK 0 # define FPU_PC_DOUBLE 0 # define FPU_PC_EXTENDED 0 # define GET_FPUCW() 0 # define SET_FPUCW(word) (void)(word) # define DECL_LONG_DOUBLE_ROUNDING # define BEGIN_LONG_DOUBLE_ROUNDING() # define END_LONG_DOUBLE_ROUNDING() #endif #endif /* _FPUCW_H */ gnuastro-0.5/bootstrapped/tests/flexmember.h0000644000175000017500000000345113217200022016300 00000000000000/* Sizes of structs with flexible array members. Copyright 2016-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . Written by Paul Eggert. */ #include /* Nonzero multiple of alignment of TYPE, suitable for FLEXSIZEOF below. On older platforms without _Alignof, use a pessimistic bound that is safe in practice even if FLEXIBLE_ARRAY_MEMBER is 1. On newer platforms, use _Alignof to get a tighter bound. */ #if !defined __STDC_VERSION__ || __STDC_VERSION__ < 201112 # define FLEXALIGNOF(type) (sizeof (type) & ~ (sizeof (type) - 1)) #else # define FLEXALIGNOF(type) _Alignof (type) #endif /* Upper bound on the size of a struct of type TYPE with a flexible array member named MEMBER that is followed by N bytes of other data. This is not simply sizeof (TYPE) + N, since it may require alignment on unusually picky C11 platforms, and FLEXIBLE_ARRAY_MEMBER may be 1 on pre-C11 platforms. Yield a value less than N if and only if arithmetic overflow occurs. */ #define FLEXSIZEOF(type, member, n) \ ((offsetof (type, member) + FLEXALIGNOF (type) - 1 + (n)) \ & ~ (FLEXALIGNOF (type) - 1)) gnuastro-0.5/bootstrapped/tests/filename.h0000644000175000017500000000365313217200022015736 00000000000000/* Basic filename support macros. Copyright (C) 2001-2004, 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _FILENAME_H #define _FILENAME_H #ifdef __cplusplus extern "C" { #endif /* Pathname support. ISSLASH(C) tests whether C is a directory separator character. IS_ABSOLUTE_PATH(P) tests whether P is an absolute path. If it is not, it may be concatenated to a directory pathname. IS_PATH_WITH_DIR(P) tests whether P contains a directory specification. */ #if defined _WIN32 || defined __WIN32__ || defined __CYGWIN__ || defined __EMX__ || defined __DJGPP__ /* Native Windows, Cygwin, OS/2, DOS */ # define ISSLASH(C) ((C) == '/' || (C) == '\\') # define HAS_DEVICE(P) \ ((((P)[0] >= 'A' && (P)[0] <= 'Z') || ((P)[0] >= 'a' && (P)[0] <= 'z')) \ && (P)[1] == ':') # define IS_ABSOLUTE_PATH(P) (ISSLASH ((P)[0]) || HAS_DEVICE (P)) # define IS_PATH_WITH_DIR(P) \ (strchr (P, '/') != NULL || strchr (P, '\\') != NULL || HAS_DEVICE (P)) # define FILE_SYSTEM_PREFIX_LEN(P) (HAS_DEVICE (P) ? 2 : 0) #else /* Unix */ # define ISSLASH(C) ((C) == '/') # define IS_ABSOLUTE_PATH(P) ISSLASH ((P)[0]) # define IS_PATH_WITH_DIR(P) (strchr (P, '/') != NULL) # define FILE_SYSTEM_PREFIX_LEN(P) 0 #endif #ifdef __cplusplus } #endif #endif /* _FILENAME_H */ gnuastro-0.5/bootstrapped/tests/fd-hook.h0000644000175000017500000001134313217200022015500 00000000000000/* Hook for making file descriptor functions close(), ioctl() extensible. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef FD_HOOK_H #define FD_HOOK_H #ifdef __cplusplus extern "C" { #endif /* Currently, this entire code is only needed for the handling of sockets on native Windows platforms. */ #if WINDOWS_SOCKETS /* Type of function that closes FD. */ typedef int (*gl_close_fn) (int fd); /* Type of function that applies a control request to FD. */ typedef int (*gl_ioctl_fn) (int fd, int request, void *arg); /* An element of the list of file descriptor hooks. In CLOS (Common Lisp Object System) speak, it consists of an "around" method for the close() function and an "around" method for the ioctl() function. The fields of this structure are considered private. */ struct fd_hook { /* Doubly linked list. */ struct fd_hook *private_next; struct fd_hook *private_prev; /* Function that treats the types of FD that it knows about and calls execute_close_hooks (REMAINING_LIST, PRIMARY, FD) as a fallback. */ int (*private_close_fn) (const struct fd_hook *remaining_list, gl_close_fn primary, int fd); /* Function that treats the types of FD that it knows about and calls execute_ioctl_hooks (REMAINING_LIST, PRIMARY, FD, REQUEST, ARG) as a fallback. */ int (*private_ioctl_fn) (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg); }; /* This type of function closes FD, applying special knowledge for the FD types it knows about, and calls execute_close_hooks (REMAINING_LIST, PRIMARY, FD) for the other FD types. In CLOS speak, REMAINING_LIST is the remaining list of "around" methods, and PRIMARY is the "primary" method for close(). */ typedef int (*close_hook_fn) (const struct fd_hook *remaining_list, gl_close_fn primary, int fd); /* Execute the close hooks in REMAINING_LIST, with PRIMARY as "primary" method. Return 0 or -1, like close() would do. */ extern int execute_close_hooks (const struct fd_hook *remaining_list, gl_close_fn primary, int fd); /* Execute all close hooks, with PRIMARY as "primary" method. Return 0 or -1, like close() would do. */ extern int execute_all_close_hooks (gl_close_fn primary, int fd); /* This type of function applies a control request to FD, applying special knowledge for the FD types it knows about, and calls execute_ioctl_hooks (REMAINING_LIST, PRIMARY, FD, REQUEST, ARG) for the other FD types. In CLOS speak, REMAINING_LIST is the remaining list of "around" methods, and PRIMARY is the "primary" method for ioctl(). */ typedef int (*ioctl_hook_fn) (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg); /* Execute the ioctl hooks in REMAINING_LIST, with PRIMARY as "primary" method. Return 0 or -1, like ioctl() would do. */ extern int execute_ioctl_hooks (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg); /* Execute all ioctl hooks, with PRIMARY as "primary" method. Return 0 or -1, like ioctl() would do. */ extern int execute_all_ioctl_hooks (gl_ioctl_fn primary, int fd, int request, void *arg); /* Add a function pair to the list of file descriptor hooks. CLOSE_HOOK and IOCTL_HOOK may be NULL, indicating no change. The LINK variable points to a piece of memory which is guaranteed to be accessible until the corresponding call to unregister_fd_hook. */ extern void register_fd_hook (close_hook_fn close_hook, ioctl_hook_fn ioctl_hook, struct fd_hook *link); /* Removes a hook from the list of file descriptor hooks. */ extern void unregister_fd_hook (struct fd_hook *link); #endif #ifdef __cplusplus } #endif #endif /* FD_HOOK_H */ gnuastro-0.5/bootstrapped/tests/fcntl.in.h0000644000175000017500000002376613217200022015700 00000000000000/* Like , but with non-working flags defined to 0. Copyright (C) 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Paul Eggert */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_system_fcntl_h /* Special invocation convention. */ /* Needed before . May also define off_t to a 64-bit type on native Windows. */ #include /* On some systems other than glibc, is a prerequisite of . On glibc systems, we would like to avoid namespace pollution. But on glibc systems, includes inside an extern "C" { ... } block, which leads to errors in C++ mode with the overridden from gnulib. These errors are known to be gone with g++ version >= 4.3. */ #if !(defined __GLIBC__ || defined __UCLIBC__) || (defined __cplusplus && defined GNULIB_NAMESPACE && (defined __ICC || !(__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 3)))) # include #endif #@INCLUDE_NEXT@ @NEXT_FCNTL_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_FCNTL_H /* Needed before . May also define off_t to a 64-bit type on native Windows. */ #include /* On some systems other than glibc, is a prerequisite of . On glibc systems, we would like to avoid namespace pollution. But on glibc systems, includes inside an extern "C" { ... } block, which leads to errors in C++ mode with the overridden from gnulib. These errors are known to be gone with g++ version >= 4.3. */ #if !(defined __GLIBC__ || defined __UCLIBC__) || (defined __cplusplus && defined GNULIB_NAMESPACE && (defined __ICC || !(__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 3)))) # include #endif /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_FCNTL_H@ #ifndef _@GUARD_PREFIX@_FCNTL_H #define _@GUARD_PREFIX@_FCNTL_H #ifndef __GLIBC__ /* Avoid namespace pollution on glibc systems. */ # include #endif /* Native Windows platforms declare open(), creat() in . */ #if (@GNULIB_OPEN@ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Declare overridden functions. */ #if @GNULIB_FCNTL@ # if @REPLACE_FCNTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fcntl # define fcntl rpl_fcntl # endif _GL_FUNCDECL_RPL (fcntl, int, (int fd, int action, ...)); _GL_CXXALIAS_RPL (fcntl, int, (int fd, int action, ...)); # else # if !@HAVE_FCNTL@ _GL_FUNCDECL_SYS (fcntl, int, (int fd, int action, ...)); # endif _GL_CXXALIAS_SYS (fcntl, int, (int fd, int action, ...)); # endif _GL_CXXALIASWARN (fcntl); #elif defined GNULIB_POSIXCHECK # undef fcntl # if HAVE_RAW_DECL_FCNTL _GL_WARN_ON_USE (fcntl, "fcntl is not always POSIX compliant - " "use gnulib module fcntl for portability"); # endif #endif #if @GNULIB_OPEN@ # if @REPLACE_OPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef open # define open rpl_open # endif _GL_FUNCDECL_RPL (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (open, int, (const char *filename, int flags, ...)); # else _GL_CXXALIAS_SYS (open, int, (const char *filename, int flags, ...)); # endif /* On HP-UX 11, in C++ mode, open() is defined as an inline function with a default argument. _GL_CXXALIASWARN does not work in this case. */ # if !defined __hpux _GL_CXXALIASWARN (open); # endif #elif defined GNULIB_POSIXCHECK # undef open /* Assume open is always declared. */ _GL_WARN_ON_USE (open, "open is not always POSIX compliant - " "use gnulib module open for portability"); #endif #if @GNULIB_OPENAT@ # if @REPLACE_OPENAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef openat # define openat rpl_openat # endif _GL_FUNCDECL_RPL (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...)); # else # if !@HAVE_OPENAT@ _GL_FUNCDECL_SYS (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (openat, int, (int fd, char const *file, int flags, /* mode_t mode */ ...)); # endif _GL_CXXALIASWARN (openat); #elif defined GNULIB_POSIXCHECK # undef openat # if HAVE_RAW_DECL_OPENAT _GL_WARN_ON_USE (openat, "openat is not portable - " "use gnulib module openat for portability"); # endif #endif /* Fix up the FD_* macros, only known to be missing on mingw. */ #ifndef FD_CLOEXEC # define FD_CLOEXEC 1 #endif /* Fix up the supported F_* macros. Intentionally leave other F_* macros undefined. Only known to be missing on mingw. */ #ifndef F_DUPFD_CLOEXEC # define F_DUPFD_CLOEXEC 0x40000000 /* Witness variable: 1 if gnulib defined F_DUPFD_CLOEXEC, 0 otherwise. */ # define GNULIB_defined_F_DUPFD_CLOEXEC 1 #else # define GNULIB_defined_F_DUPFD_CLOEXEC 0 #endif #ifndef F_DUPFD # define F_DUPFD 1 #endif #ifndef F_GETFD # define F_GETFD 2 #endif /* Fix up the O_* macros. */ /* AIX 7.1 with XL C 12.1 defines O_CLOEXEC, O_NOFOLLOW, and O_TTY_INIT to values outside 'int' range, so omit these misdefinitions. But avoid namespace pollution on non-AIX systems. */ #ifdef _AIX # include # if defined O_CLOEXEC && ! (INT_MIN <= O_CLOEXEC && O_CLOEXEC <= INT_MAX) # undef O_CLOEXEC # endif # if defined O_NOFOLLOW && ! (INT_MIN <= O_NOFOLLOW && O_NOFOLLOW <= INT_MAX) # undef O_NOFOLLOW # endif # if defined O_TTY_INIT && ! (INT_MIN <= O_TTY_INIT && O_TTY_INIT <= INT_MAX) # undef O_TTY_INIT # endif #endif #if !defined O_DIRECT && defined O_DIRECTIO /* Tru64 spells it 'O_DIRECTIO'. */ # define O_DIRECT O_DIRECTIO #endif #if !defined O_CLOEXEC && defined O_NOINHERIT /* Mingw spells it 'O_NOINHERIT'. */ # define O_CLOEXEC O_NOINHERIT #endif #ifndef O_CLOEXEC # define O_CLOEXEC 0x40000000 /* Try to not collide with system O_* flags. */ # define GNULIB_defined_O_CLOEXEC 1 #else # define GNULIB_defined_O_CLOEXEC 0 #endif #ifndef O_DIRECT # define O_DIRECT 0 #endif #ifndef O_DIRECTORY # define O_DIRECTORY 0 #endif #ifndef O_DSYNC # define O_DSYNC 0 #endif #ifndef O_EXEC # define O_EXEC O_RDONLY /* This is often close enough in older systems. */ #endif #ifndef O_IGNORE_CTTY # define O_IGNORE_CTTY 0 #endif #ifndef O_NDELAY # define O_NDELAY 0 #endif #ifndef O_NOATIME # define O_NOATIME 0 #endif #ifndef O_NONBLOCK # define O_NONBLOCK O_NDELAY #endif /* If the gnulib module 'nonblocking' is in use, guarantee a working non-zero value of O_NONBLOCK. Otherwise, O_NONBLOCK is defined (above) to O_NDELAY or to 0 as fallback. */ #if @GNULIB_NONBLOCKING@ # if O_NONBLOCK # define GNULIB_defined_O_NONBLOCK 0 # else # define GNULIB_defined_O_NONBLOCK 1 # undef O_NONBLOCK # define O_NONBLOCK 0x40000000 # endif #endif #ifndef O_NOCTTY # define O_NOCTTY 0 #endif #ifndef O_NOFOLLOW # define O_NOFOLLOW 0 #endif #ifndef O_NOLINK # define O_NOLINK 0 #endif #ifndef O_NOLINKS # define O_NOLINKS 0 #endif #ifndef O_NOTRANS # define O_NOTRANS 0 #endif #ifndef O_RSYNC # define O_RSYNC 0 #endif #ifndef O_SEARCH # define O_SEARCH O_RDONLY /* This is often close enough in older systems. */ #endif #ifndef O_SYNC # define O_SYNC 0 #endif #ifndef O_TTY_INIT # define O_TTY_INIT 0 #endif #if ~O_ACCMODE & (O_RDONLY | O_WRONLY | O_RDWR | O_EXEC | O_SEARCH) # undef O_ACCMODE # define O_ACCMODE (O_RDONLY | O_WRONLY | O_RDWR | O_EXEC | O_SEARCH) #endif /* For systems that distinguish between text and binary I/O. O_BINARY is usually declared in fcntl.h */ #if !defined O_BINARY && defined _O_BINARY /* For MSC-compatible compilers. */ # define O_BINARY _O_BINARY # define O_TEXT _O_TEXT #endif #if defined __BEOS__ || defined __HAIKU__ /* BeOS 5 and Haiku have O_BINARY and O_TEXT, but they have no effect. */ # undef O_BINARY # undef O_TEXT #endif #ifndef O_BINARY # define O_BINARY 0 # define O_TEXT 0 #endif /* Fix up the AT_* macros. */ /* Work around a bug in Solaris 9 and 10: AT_FDCWD is positive. Its value exceeds INT_MAX, so its use as an int doesn't conform to the C standard, and GCC and Sun C complain in some cases. If the bug is present, undef AT_FDCWD here, so it can be redefined below. */ #if 0 < AT_FDCWD && AT_FDCWD == 0xffd19553 # undef AT_FDCWD #endif /* Use the same bit pattern as Solaris 9, but with the proper signedness. The bit pattern is important, in case this actually is Solaris with the above workaround. */ #ifndef AT_FDCWD # define AT_FDCWD (-3041965) #endif /* Use the same values as Solaris 9. This shouldn't matter, but there's no real reason to differ. */ #ifndef AT_SYMLINK_NOFOLLOW # define AT_SYMLINK_NOFOLLOW 4096 #endif #ifndef AT_REMOVEDIR # define AT_REMOVEDIR 1 #endif /* Solaris 9 lacks these two, so just pick unique values. */ #ifndef AT_SYMLINK_FOLLOW # define AT_SYMLINK_FOLLOW 2 #endif #ifndef AT_EACCESS # define AT_EACCESS 4 #endif #endif /* _@GUARD_PREFIX@_FCNTL_H */ #endif /* _@GUARD_PREFIX@_FCNTL_H */ #endif gnuastro-0.5/bootstrapped/tests/ctype.in.h0000644000175000017500000000342213217200022015701 00000000000000/* A substitute for ISO C99 , for platforms on which it is incomplete. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible. */ /* * ISO C 99 for platforms on which it is incomplete. * */ #ifndef _@GUARD_PREFIX@_CTYPE_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Include the original . */ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_CTYPE_H@ #ifndef _@GUARD_PREFIX@_CTYPE_H #define _@GUARD_PREFIX@_CTYPE_H /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Return non-zero if c is a blank, i.e. a space or tab character. */ #if @GNULIB_ISBLANK@ # if !@HAVE_ISBLANK@ _GL_EXTERN_C int isblank (int c); # endif #elif defined GNULIB_POSIXCHECK # undef isblank # if HAVE_RAW_DECL_ISBLANK _GL_WARN_ON_USE (isblank, "isblank is unportable - " "use gnulib module isblank for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_CTYPE_H */ #endif /* _@GUARD_PREFIX@_CTYPE_H */ gnuastro-0.5/bootstrapped/tests/cloexec.h0000644000175000017500000000273413217200022015577 00000000000000/* cloexec.c - set or clear the close-on-exec descriptor flag Copyright (C) 2004, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Set the 'FD_CLOEXEC' flag of DESC if VALUE is true, or clear the flag if VALUE is false. Return 0 on success, or -1 on error with 'errno' set. Note that on MingW, this function does NOT protect DESC from being inherited into spawned children. Instead, either use dup_cloexec followed by closing the original DESC, or use interfaces such as open or pipe2 that accept flags like O_CLOEXEC to create DESC non-inheritable in the first place. */ int set_cloexec_flag (int desc, bool value); /* Duplicates a file handle FD, while marking the copy to be closed prior to exec or spawn. Returns -1 and sets errno if FD could not be duplicated. */ int dup_cloexec (int fd); gnuastro-0.5/bootstrapped/tests/test-c-strcase.sh0000755000175000017500000000114313217200023017176 00000000000000#!/bin/sh # Test in the C locale. ./test-c-strcasecmp${EXEEXT} || exit 1 ./test-c-strncasecmp${EXEEXT} || exit 1 # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR != none; then LC_ALL=$LOCALE_FR ./test-c-strcasecmp${EXEEXT} locale || exit 1 LC_ALL=$LOCALE_FR ./test-c-strncasecmp${EXEEXT} locale || exit 1 fi # Test in a Turkish UTF-8 locale. : ${LOCALE_TR_UTF8=tr_TR.UTF-8} if test $LOCALE_TR_UTF8 != none; then LC_ALL=$LOCALE_TR_UTF8 ./test-c-strcasecmp${EXEEXT} locale || exit 1 LC_ALL=$LOCALE_TR_UTF8 ./test-c-strncasecmp${EXEEXT} locale || exit 1 fi exit 0 gnuastro-0.5/bootstrapped/tests/test-btowc2.sh0000755000175000017500000000056613217200023016522 00000000000000#!/bin/sh # Test whether a specific UTF-8 locale is installed. : ${LOCALE_FR_UTF8=fr_FR.UTF-8} if test $LOCALE_FR_UTF8 = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no french Unicode locale is installed" else echo "Skipping test: no french Unicode locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR_UTF8 \ ./test-btowc${EXEEXT} 2 gnuastro-0.5/bootstrapped/tests/test-btowc1.sh0000755000175000017500000000054313217200023016514 00000000000000#!/bin/sh # Test in an ISO-8859-1 or ISO-8859-15 locale. : ${LOCALE_FR=fr_FR} if test $LOCALE_FR = none; then if test -f /usr/bin/localedef; then echo "Skipping test: no traditional french locale is installed" else echo "Skipping test: no traditional french locale is supported" fi exit 77 fi LC_ALL=$LOCALE_FR \ ./test-btowc${EXEEXT} 1 gnuastro-0.5/bootstrapped/tests/test-binary-io.sh0000755000175000017500000000036513217200023017210 00000000000000#!/bin/sh tmpfiles="" trap 'rm -fr $tmpfiles' 1 2 3 15 tmpfiles="$tmpfiles t-bin-out0.tmp t-bin-out1.tmp" ./test-binary-io${EXEEXT} 1 > t-bin-out1.tmp || exit 1 cmp t-bin-out0.tmp t-bin-out1.tmp > /dev/null || exit 1 rm -fr $tmpfiles exit 0 gnuastro-0.5/bootstrapped/tests/arpa_inet.in.h0000644000175000017500000001143413217200022016521 00000000000000/* A GNU-like . Copyright (C) 2005-2006, 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_ARPA_INET_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if @HAVE_FEATURES_H@ # include /* for __GLIBC__ */ #endif /* Gnulib's sys/socket.h is responsible for defining socklen_t (used below) and for pulling in winsock2.h etc. under MinGW. But avoid namespace pollution on glibc systems. */ #ifndef __GLIBC__ # include #endif /* On NonStop Kernel, inet_ntop and inet_pton are declared in . But avoid namespace pollution on glibc systems. */ #if defined __TANDEM && !defined __GLIBC__ # include #endif #if @HAVE_ARPA_INET_H@ /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_ARPA_INET_H@ #endif #ifndef _@GUARD_PREFIX@_ARPA_INET_H #define _@GUARD_PREFIX@_ARPA_INET_H /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #if @GNULIB_INET_NTOP@ /* Converts an internet address from internal format to a printable, presentable format. AF is an internet address family, such as AF_INET or AF_INET6. SRC points to a 'struct in_addr' (for AF_INET) or 'struct in6_addr' (for AF_INET6). DST points to a buffer having room for CNT bytes. The printable representation of the address (in numeric form, not surrounded by [...], no reverse DNS is done) is placed in DST, and DST is returned. If an error occurs, the return value is NULL and errno is set. If CNT bytes are not sufficient to hold the result, the return value is NULL and errno is set to ENOSPC. A good value for CNT is 46. For more details, see the POSIX:2001 specification . */ # if @REPLACE_INET_NTOP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef inet_ntop # define inet_ntop rpl_inet_ntop # endif _GL_FUNCDECL_RPL (inet_ntop, const char *, (int af, const void *restrict src, char *restrict dst, socklen_t cnt) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (inet_ntop, const char *, (int af, const void *restrict src, char *restrict dst, socklen_t cnt)); # else # if !@HAVE_DECL_INET_NTOP@ _GL_FUNCDECL_SYS (inet_ntop, const char *, (int af, const void *restrict src, char *restrict dst, socklen_t cnt) _GL_ARG_NONNULL ((2, 3))); # endif /* Need to cast, because on NonStop Kernel, the fourth parameter is size_t cnt. */ _GL_CXXALIAS_SYS_CAST (inet_ntop, const char *, (int af, const void *restrict src, char *restrict dst, socklen_t cnt)); # endif _GL_CXXALIASWARN (inet_ntop); #elif defined GNULIB_POSIXCHECK # undef inet_ntop # if HAVE_RAW_DECL_INET_NTOP _GL_WARN_ON_USE (inet_ntop, "inet_ntop is unportable - " "use gnulib module inet_ntop for portability"); # endif #endif #if @GNULIB_INET_PTON@ # if @REPLACE_INET_PTON@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef inet_pton # define inet_pton rpl_inet_pton # endif _GL_FUNCDECL_RPL (inet_pton, int, (int af, const char *restrict src, void *restrict dst) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (inet_pton, int, (int af, const char *restrict src, void *restrict dst)); # else # if !@HAVE_DECL_INET_PTON@ _GL_FUNCDECL_SYS (inet_pton, int, (int af, const char *restrict src, void *restrict dst) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (inet_pton, int, (int af, const char *restrict src, void *restrict dst)); # endif _GL_CXXALIASWARN (inet_pton); #elif defined GNULIB_POSIXCHECK # undef inet_pton # if HAVE_RAW_DECL_INET_PTON _GL_WARN_ON_USE (inet_pton, "inet_pton is unportable - " "use gnulib module inet_pton for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_ARPA_INET_H */ #endif /* _@GUARD_PREFIX@_ARPA_INET_H */ gnuastro-0.5/bootstrapped/tests/test-argp-2.sh0000755000175000017500000000651413217200023016411 00000000000000#! /bin/sh # Test suite for argp. # Copyright (C) 2006-2017 Free Software Foundation, Inc. # This file is part of the GNUlib Library. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . */ TMP=argp.$$ unset ARGP_HELP_FMT ERR=0 func_compare() { # If argp was compiled without base_name, it will display full program name. # If run on mingw, it will display the program name with a .exe suffix. sed '1{ s,: [^ ]*/test-argp,: test-argp, s,: test-argp\.exe,: test-argp, }' | LC_ALL=C tr -d '\r' | diff -c $TMP - } #### # Test --usage output cat > $TMP < $TMP <$TMP <. EOT # Compare --help output, but filter out any bug-reporting email address. ./test-argp$EXEEXT --help \ | sed 's/^\(Report bugs to \)<[^>]*>.$/\1<>./' | func_compare || ERR=1 #### # Test ambiguous option handling ./test-argp$EXEEXT --optio 2>/dev/null && ERR=1 #### # Run built-in tests ./test-argp$EXEEXT || ERR=1 rm $TMP exit $ERR gnuastro-0.5/bootstrapped/tests/macros.h0000644000175000017500000000673113217200023015443 00000000000000/* Common macros used by gnulib tests. Copyright (C) 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This file contains macros that are used by many gnulib tests. Put here only frequently used macros, say, used by 10 tests or more. */ #include #include #ifndef FALLTHROUGH # if __GNUC__ < 7 # define FALLTHROUGH ((void) 0) # else # define FALLTHROUGH __attribute__ ((__fallthrough__)) # endif #endif /* Define ASSERT_STREAM before including this file if ASSERT must target a stream other than stderr. */ #ifndef ASSERT_STREAM # define ASSERT_STREAM stderr #endif /* ASSERT (condition); verifies that the specified condition is fulfilled. If not, a message is printed to ASSERT_STREAM if defined (defaulting to stderr if undefined) and the program is terminated with an error code. This macro has the following properties: - The programmer specifies the expected condition, not the failure condition. This simplifies thinking. - The condition is tested always, regardless of compilation flags. (Unlike the macro from .) - On Unix platforms, the tester can debug the test program with a debugger (provided core dumps are enabled: "ulimit -c unlimited"). - For the sake of platforms where no debugger is available (such as some mingw systems), an error message is printed on the error stream that includes the source location of the ASSERT invocation. */ #define ASSERT(expr) \ do \ { \ if (!(expr)) \ { \ fprintf (ASSERT_STREAM, "%s:%d: assertion '%s' failed\n", \ __FILE__, __LINE__, #expr); \ fflush (ASSERT_STREAM); \ abort (); \ } \ } \ while (0) /* SIZEOF (array) returns the number of elements of an array. It works for arrays that are declared outside functions and for local variables of array type. It does *not* work for function parameters of array type, because they are actually parameters of pointer type. */ #define SIZEOF(array) (sizeof (array) / sizeof (array[0])) /* STREQ (str1, str2) Return true if two strings compare equal. */ #define STREQ(a, b) (strcmp (a, b) == 0) /* Some numbers in the interval [0,1). */ extern const float randomf[1000]; extern const double randomd[1000]; extern const long double randoml[1000]; gnuastro-0.5/bootstrapped/tests/signature.h0000644000175000017500000000367713217200023016166 00000000000000/* Macro for checking that a function declaration is compliant. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef SIGNATURE_CHECK /* Check that the function FN takes the specified arguments ARGS with a return type of RET. This header is designed to be included after and the one system header that is supposed to contain the function being checked, but prior to any other system headers that are necessary for the unit test. Therefore, this file does not include any system headers, nor reference anything outside of the macro arguments. For an example, if foo.h should provide: extern int foo (char, float); then the unit test named test-foo.c would start out with: #include #include #include "signature.h" SIGNATURE_CHECK (foo, int, (char, float)); #include ... */ # define SIGNATURE_CHECK(fn, ret, args) \ SIGNATURE_CHECK1 (fn, ret, args, __LINE__) /* Necessary to allow multiple SIGNATURE_CHECK lines in a unit test. Note that the checks must not occupy the same line. */ # define SIGNATURE_CHECK1(fn, ret, args, id) \ SIGNATURE_CHECK2 (fn, ret, args, id) /* macroexpand line */ # define SIGNATURE_CHECK2(fn, ret, args, id) \ static ret (* _GL_UNUSED signature_check ## id) args = fn #endif /* SIGNATURE_CHECK */ gnuastro-0.5/bootstrapped/tests/w32sock.h0000644000175000017500000000643113217200024015450 00000000000000/* w32sock.h --- internal auxiliary functions for Windows socket functions Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include /* Get O_RDWR and O_BINARY. */ #include /* Get _open_osfhandle(). */ #include /* Get _get_osfhandle(). */ #if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" #else # include #endif #define FD_TO_SOCKET(fd) ((SOCKET) _get_osfhandle ((fd))) #define SOCKET_TO_FD(fh) (_open_osfhandle ((intptr_t) (fh), O_RDWR | O_BINARY)) static inline void set_winsock_errno (void) { int err = WSAGetLastError (); /* Map some WSAE* errors to the runtime library's error codes. */ switch (err) { case WSA_INVALID_HANDLE: errno = EBADF; break; case WSA_NOT_ENOUGH_MEMORY: errno = ENOMEM; break; case WSA_INVALID_PARAMETER: errno = EINVAL; break; case WSAENAMETOOLONG: errno = ENAMETOOLONG; break; case WSAENOTEMPTY: errno = ENOTEMPTY; break; case WSAEWOULDBLOCK: errno = EWOULDBLOCK; break; case WSAEINPROGRESS: errno = EINPROGRESS; break; case WSAEALREADY: errno = EALREADY; break; case WSAENOTSOCK: errno = ENOTSOCK; break; case WSAEDESTADDRREQ: errno = EDESTADDRREQ; break; case WSAEMSGSIZE: errno = EMSGSIZE; break; case WSAEPROTOTYPE: errno = EPROTOTYPE; break; case WSAENOPROTOOPT: errno = ENOPROTOOPT; break; case WSAEPROTONOSUPPORT: errno = EPROTONOSUPPORT; break; case WSAEOPNOTSUPP: errno = EOPNOTSUPP; break; case WSAEAFNOSUPPORT: errno = EAFNOSUPPORT; break; case WSAEADDRINUSE: errno = EADDRINUSE; break; case WSAEADDRNOTAVAIL: errno = EADDRNOTAVAIL; break; case WSAENETDOWN: errno = ENETDOWN; break; case WSAENETUNREACH: errno = ENETUNREACH; break; case WSAENETRESET: errno = ENETRESET; break; case WSAECONNABORTED: errno = ECONNABORTED; break; case WSAECONNRESET: errno = ECONNRESET; break; case WSAENOBUFS: errno = ENOBUFS; break; case WSAEISCONN: errno = EISCONN; break; case WSAENOTCONN: errno = ENOTCONN; break; case WSAETIMEDOUT: errno = ETIMEDOUT; break; case WSAECONNREFUSED: errno = ECONNREFUSED; break; case WSAELOOP: errno = ELOOP; break; case WSAEHOSTUNREACH: errno = EHOSTUNREACH; break; default: errno = (err > 10000 && err < 10025) ? err - 10000 : err; break; } } gnuastro-0.5/bootstrapped/tests/test-wcwidth.c0000644000175000017500000000507313217200024016577 00000000000000/* Test of wcwidth() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (wcwidth, int, (wchar_t)); #include #include #include "c-ctype.h" #include "localcharset.h" #include "macros.h" int main () { wchar_t wc; #ifdef C_CTYPE_ASCII /* Test width of ASCII characters. */ for (wc = 0x20; wc < 0x7F; wc++) ASSERT (wcwidth (wc) == 1); #endif /* Switch to an UTF-8 locale. */ if (setlocale (LC_ALL, "fr_FR.UTF-8") != NULL /* Check whether it's really an UTF-8 locale. On OpenBSD 4.0, the setlocale call succeeds only for the LC_CTYPE category and therefore returns "C/fr_FR.UTF-8/C/C/C/C", but the LC_CTYPE category is effectively set to an ASCII LC_CTYPE category; in particular, locale_charset() returns "ASCII". */ && strcmp (locale_charset (), "UTF-8") == 0) { /* Test width of ASCII characters. */ for (wc = 0x20; wc < 0x7F; wc++) ASSERT (wcwidth (wc) == 1); /* Test width of some non-spacing characters. */ ASSERT (wcwidth (0x0301) == 0); ASSERT (wcwidth (0x05B0) == 0); /* Test width of some format control characters. */ ASSERT (wcwidth (0x200E) <= 0); ASSERT (wcwidth (0x2060) <= 0); #if 0 /* wchar_t may be only 16 bits. */ ASSERT (wcwidth (0xE0001) <= 0); ASSERT (wcwidth (0xE0044) <= 0); #endif /* Test width of some zero width characters. */ ASSERT (wcwidth (0x200B) == 0); ASSERT (wcwidth (0xFEFF) <= 0); /* Test width of some CJK characters. */ ASSERT (wcwidth (0x3000) == 2); ASSERT (wcwidth (0xB250) == 2); ASSERT (wcwidth (0xFF1A) == 2); #if 0 /* wchar_t may be only 16 bits. */ ASSERT (wcwidth (0x20369) == 2); ASSERT (wcwidth (0x2F876) == 2); #endif } return 0; } gnuastro-0.5/bootstrapped/tests/test-wctype-h.c0000644000175000017500000000376613217200024016675 00000000000000/* Test of substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "macros.h" /* Check that the type wint_t is defined. */ wint_t a = 'x'; /* Check that WEOF is defined. */ wint_t e = WEOF; /* Check that the type wctype_t is defined. */ wctype_t p; /* Check that the type wctrans_t is defined. */ wctrans_t q; int main (void) { /* Check that the isw* functions exist as functions or as macros. */ (void) iswalnum (0); (void) iswalpha (0); (void) iswcntrl (0); (void) iswdigit (0); (void) iswgraph (0); (void) iswlower (0); (void) iswprint (0); (void) iswpunct (0); (void) iswspace (0); (void) iswupper (0); (void) iswxdigit (0); /* Check that the isw* functions map WEOF to 0. */ ASSERT (!iswalnum (e)); ASSERT (!iswalpha (e)); ASSERT (!iswcntrl (e)); ASSERT (!iswdigit (e)); ASSERT (!iswgraph (e)); ASSERT (!iswlower (e)); ASSERT (!iswprint (e)); ASSERT (!iswpunct (e)); ASSERT (!iswspace (e)); ASSERT (!iswupper (e)); ASSERT (!iswxdigit (e)); /* Check that the tow* functions exist as functions or as macros. */ (void) towlower (0); (void) towupper (0); /* Check that the tow* functions map WEOF to WEOF. */ ASSERT (towlower (e) == e); ASSERT (towupper (e) == e); return 0; } gnuastro-0.5/bootstrapped/tests/test-wcrtomb-w32.c0000644000175000017500000002171613217200024017216 00000000000000/* Test of conversion of wide character to multibyte character. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include #include "macros.h" #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ static int test_one_locale (const char *name, int codepage) { char buf[64]; size_t ret; # if 1 /* Portable code to set the locale. */ { char name_with_codepage[1024]; sprintf (name_with_codepage, "%s.%d", name, codepage); /* Set the locale. */ if (setlocale (LC_ALL, name_with_codepage) == NULL) return 77; } # else /* Hacky way to set a locale.codepage combination that setlocale() refuses to set. */ { /* Codepage of the current locale, set with setlocale(). Not necessarily the same as GetACP(). */ extern __declspec(dllimport) unsigned int __lc_codepage; /* Set the locale. */ if (setlocale (LC_ALL, name) == NULL) return 77; /* Clobber the codepage and MB_CUR_MAX, both set by setlocale(). */ __lc_codepage = codepage; switch (codepage) { case 1252: case 1256: MB_CUR_MAX = 1; break; case 932: case 950: case 936: MB_CUR_MAX = 2; break; case 54936: case 65001: MB_CUR_MAX = 4; break; } /* Test whether the codepage is really available. */ { mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, " ", 1, &state) == (size_t)(-1)) return 77; } } # endif /* Test NUL character. */ { buf[0] = 'x'; ret = wcrtomb (buf, 0, NULL); ASSERT (ret == 1); ASSERT (buf[0] == '\0'); } /* Test single bytes. */ { int c; for (c = 0; c < 0x100; c++) switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set". */ ret = wcrtomb (buf, btowc (c), NULL); ASSERT (ret == 1); ASSERT (buf[0] == (char) c); break; } } /* Test special calling convention, passing a NULL pointer. */ { ret = wcrtomb (NULL, '\0', NULL); ASSERT (ret == 1); ret = wcrtomb (NULL, btowc ('x'), NULL); ASSERT (ret == 1); } switch (codepage) { case 1252: /* Locale encoding is CP1252, an extension of ISO-8859-1. */ { /* Convert "B\374\337er": "Büßer" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00FC, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\374", 1) == 0); ASSERT (buf[1] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00DF, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\337", 1) == 0); ASSERT (buf[1] == 'x'); } return 0; case 1256: /* Locale encoding is CP1256, not the same as ISO-8859-6. */ { /* Convert "x\302\341\346y": "xآلوy" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x0622, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\302", 1) == 0); ASSERT (buf[1] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x0644, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\341", 1) == 0); ASSERT (buf[1] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x0648, NULL); ASSERT (ret == 1); ASSERT (memcmp (buf, "\346", 1) == 0); ASSERT (buf[1] == 'x'); } return 0; case 932: /* Locale encoding is CP932, similar to Shift_JIS. */ { /* Convert "<\223\372\226\173\214\352>": "<日本語>" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x65E5, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\223\372", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x672C, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\226\173", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x8A9E, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\214\352", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; case 950: /* Locale encoding is CP950, similar to Big5. */ { /* Convert "<\244\351\245\273\273\171>": "<日本語>" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x65E5, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\244\351", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x672C, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\245\273", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x8A9E, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\273\171", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; case 936: /* Locale encoding is CP936 = GBK, an extension of GB2312. */ { /* Convert "<\310\325\261\276\325\132>": "<日本語>" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x65E5, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\310\325", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x672C, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\261\276", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x8A9E, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\325\132", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; case 54936: /* Locale encoding is CP54936 = GB18030. */ { /* Convert "B\250\271\201\060\211\070er": "Büßer" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00FC, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\250\271", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00DF, NULL); ASSERT (ret == 4); ASSERT (memcmp (buf, "\201\060\211\070", 4) == 0); ASSERT (buf[4] == 'x'); } return 0; case 65001: /* Locale encoding is CP65001 = UTF-8. */ { /* Convert "B\303\274\303\237er": "Büßer" */ memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00FC, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\303\274", 2) == 0); ASSERT (buf[2] == 'x'); memset (buf, 'x', 8); ret = wcrtomb (buf, 0x00DF, NULL); ASSERT (ret == 2); ASSERT (memcmp (buf, "\303\237", 2) == 0); ASSERT (buf[2] == 'x'); } return 0; default: return 1; } } int main (int argc, char *argv[]) { int codepage = atoi (argv[argc - 1]); int result; int i; result = 77; for (i = 1; i < argc - 1; i++) { int ret = test_one_locale (argv[i], codepage); if (ret != 77) result = ret; } if (result == 77) { fprintf (stderr, "Skipping test: found no locale with codepage %d\n", codepage); } return result; } #else int main (int argc, char *argv[]) { fputs ("Skipping test: not a native Windows system\n", stderr); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-wcrtomb.c0000644000175000017500000001101713217200024016576 00000000000000/* Test of conversion of wide character to multibyte character. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (wcrtomb, size_t, (char *, wchar_t, mbstate_t *)); #include #include #include #include "macros.h" /* Check the multibyte character s[0..n-1]. */ static void check_character (const char *s, size_t n) { wchar_t wc; char buf[64]; int iret; size_t ret; wc = (wchar_t) 0xBADFACE; iret = mbtowc (&wc, s, n); ASSERT (iret == n); ret = wcrtomb (buf, wc, NULL); ASSERT (ret == n); ASSERT (memcmp (buf, s, n) == 0); /* Test special calling convention, passing a NULL pointer. */ ret = wcrtomb (NULL, wc, NULL); ASSERT (ret == 1); } int main (int argc, char *argv[]) { char buf[64]; size_t ret; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; /* Test NUL character. */ { buf[0] = 'x'; ret = wcrtomb (buf, 0, NULL); ASSERT (ret == 1); ASSERT (buf[0] == '\0'); } /* Test single bytes. */ { int c; for (c = 0; c < 0x100; c++) switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set". */ ret = wcrtomb (buf, btowc (c), NULL); ASSERT (ret == 1); ASSERT (buf[0] == (char) c); break; } } /* Test special calling convention, passing a NULL pointer. */ { ret = wcrtomb (NULL, '\0', NULL); ASSERT (ret == 1); ret = wcrtomb (NULL, btowc ('x'), NULL); ASSERT (ret == 1); } if (argc > 1) switch (argv[1][0]) { case '1': /* Locale encoding is ISO-8859-1 or ISO-8859-15. */ { const char input[] = "B\374\337er"; /* "Büßer" */ check_character (input + 1, 1); check_character (input + 2, 1); } return 0; case '2': /* Locale encoding is UTF-8. */ { const char input[] = "B\303\274\303\237er"; /* "Büßer" */ check_character (input + 1, 2); check_character (input + 3, 2); } return 0; case '3': /* Locale encoding is EUC-JP. */ { const char input[] = "<\306\374\313\334\270\354>"; /* "<日本語>" */ check_character (input + 1, 2); check_character (input + 3, 2); check_character (input + 5, 2); } return 0; case '4': /* Locale encoding is GB18030. */ { const char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ check_character (input + 1, 2); check_character (input + 3, 4); } return 0; } return 1; } gnuastro-0.5/bootstrapped/tests/test-wchar.c0000644000175000017500000000213613217200024016227 00000000000000/* Test of substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that the types wchar_t and wint_t are defined. */ wchar_t a = 'c'; wint_t b = 'x'; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-vsnprintf.c0000644000175000017500000000430513217200024017154 00000000000000/* Test of vsnprintf() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (vsnprintf, int, (char *, size_t, char const *, va_list)); #include #include #include "macros.h" static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } int main (int argc, char *argv[]) { char buf[8]; int size; int retval; retval = my_snprintf (NULL, 0, "%d", 12345); ASSERT (retval == 5); for (size = 0; size <= 8; size++) { memcpy (buf, "DEADBEEF", 8); retval = my_snprintf (buf, size, "%d", 12345); ASSERT (retval == 5); if (size < 6) { if (size > 0) { ASSERT (memcmp (buf, "12345", size - 1) == 0); ASSERT (buf[size - 1] == '\0' || buf[size - 1] == '0' + size); } #if !CHECK_VSNPRINTF_POSIX if (size > 0) #endif ASSERT (memcmp (buf + size, &"DEADBEEF"[size], 8 - size) == 0); } else { ASSERT (memcmp (buf, "12345\0EF", 8) == 0); } } /* Test the support of the POSIX/XSI format strings with positions. */ { char result[100]; retval = my_snprintf (result, sizeof (result), "%2$d %1$d", 33, 55); ASSERT (strcmp (result, "55 33") == 0); ASSERT (retval == strlen (result)); } return 0; } gnuastro-0.5/bootstrapped/tests/test-verify-try.c0000644000175000017500000000161313217200024017242 00000000000000/* Test the "verify" module. Copyright (C) 2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This is a separate source file, so that the execution of test-verify.sh does not interfere with the building of the 'test-verify' program. */ #include "test-verify.c" gnuastro-0.5/bootstrapped/tests/test-verify.c0000644000175000017500000000350413217200024016427 00000000000000/* Test the "verify" module. Copyright (C) 2005, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible. */ #include #include "verify.h" #ifndef EXP_FAIL # define EXP_FAIL 0 #endif int x; enum { a, b, c }; #if EXP_FAIL == 1 verify (x >= 0); /* should give ERROR: non-constant expression */ #endif verify (c == 2); /* should be ok */ #if EXP_FAIL == 2 verify (1 + 1 == 3); /* should give ERROR */ #endif verify (1 == 1); verify (1 == 1); /* should be ok */ enum { item = verify_true (1 == 1) * 0 + 17 /* should be ok */ }; static int function (int n) { #if EXP_FAIL == 3 verify (n >= 0); /* should give ERROR: non-constant expression */ #endif verify (c == 2); /* should be ok */ #if EXP_FAIL == 4 verify (1 + 1 == 3); /* should give ERROR */ #endif verify (1 == 1); verify (1 == 1); /* should be ok */ if (n) return ((void) verify_expr (1 == 1, 1), verify_expr (1 == 1, 8)); /* should be ok */ #if EXP_FAIL == 5 return verify_expr (1 == 2, 5); /* should give ERROR */ #endif return 0; } int main (void) { return !(function (0) == 0 && function (1) == 8); } gnuastro-0.5/bootstrapped/tests/test-vasnprintf.c0000644000175000017500000000433613217200024017321 00000000000000/* Test of vasnprintf() and asnprintf() functions. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "vasnprintf.h" #include #include #include #include "macros.h" static void test_function (char * (*my_asnprintf) (char *, size_t *, const char *, ...)) { char buf[8]; int size; for (size = 0; size <= 8; size++) { size_t length = size; char *result = my_asnprintf (NULL, &length, "%d", 12345); ASSERT (result != NULL); ASSERT (strcmp (result, "12345") == 0); ASSERT (length == 5); free (result); } for (size = 0; size <= 8; size++) { size_t length; char *result; memcpy (buf, "DEADBEEF", 8); length = size; result = my_asnprintf (buf, &length, "%d", 12345); ASSERT (result != NULL); ASSERT (strcmp (result, "12345") == 0); ASSERT (length == 5); if (size < 6) ASSERT (result != buf); ASSERT (memcmp (buf + size, &"DEADBEEF"[size], 8 - size) == 0); if (result != buf) free (result); } } static char * my_asnprintf (char *resultbuf, size_t *lengthp, const char *format, ...) { va_list args; char *ret; va_start (args, format); ret = vasnprintf (resultbuf, lengthp, format, args); va_end (args); return ret; } static void test_vasnprintf () { test_function (my_asnprintf); } static void test_asnprintf () { test_function (asnprintf); } int main (int argc, char *argv[]) { test_vasnprintf (); test_asnprintf (); return 0; } gnuastro-0.5/bootstrapped/tests/test-usleep.c0000644000175000017500000000211213217200024016412 00000000000000/* Test of usleep() function. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (usleep, int, (useconds_t)); #include #include "macros.h" int main (void) { time_t start = time (NULL); ASSERT (usleep (1000000) == 0); ASSERT (start < time (NULL)); ASSERT (usleep (0) == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-unsetenv.c0000644000175000017500000000337613217200024017001 00000000000000/* Tests of unsetenv. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (unsetenv, int, (char const *)); #include #include #include #include "macros.h" int main (void) { char entry[] = "b=2"; /* Test removal when multiple entries present. */ ASSERT (putenv ((char *) "a=1") == 0); ASSERT (putenv (entry) == 0); entry[0] = 'a'; /* Unspecified what getenv("a") would be at this point. */ ASSERT (unsetenv ("a") == 0); /* Both entries will be removed. */ ASSERT (getenv ("a") == NULL); ASSERT (unsetenv ("a") == 0); /* Required to fail with EINVAL. */ errno = 0; ASSERT (unsetenv ("") == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (unsetenv ("a=b") == -1); ASSERT (errno == EINVAL); #if 0 /* glibc and gnulib's implementation guarantee this, but POSIX no longer requires it: http://austingroupbugs.net/view.php?id=185 */ errno = 0; ASSERT (unsetenv (NULL) == -1); ASSERT (errno == EINVAL); #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-unistd.c0000644000175000017500000000305013217200024016425 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); /* Check that the various SEEK_* macros are defined. */ int sk[] = { SEEK_CUR, SEEK_END, SEEK_SET }; /* Check that the various *_FILENO macros are defined. */ #if ! (defined STDIN_FILENO \ && (STDIN_FILENO + STDOUT_FILENO + STDERR_FILENO == 3)) missing or broken *_FILENO macros #endif /* Check that the types are all defined. */ size_t t1; ssize_t t2; #ifdef TODO /* Not implemented in gnulib yet */ uid_t t3; gid_t t4; #endif off_t t5; pid_t t6; #ifdef TODO useconds_t t7; intptr_t t8; #endif int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-time.c0000644000175000017500000000236113217200024016061 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that the types are all defined. */ struct timespec t1; #if 0 /* POSIX:2008 does not require pid_t in unconditionally, and indeed it's missing on Mac OS X 10.5, FreeBSD 6.4, OpenBSD 4.9, mingw. */ pid_t t2; #endif /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-thread_self.c0000644000175000017500000000215113217200024017400 00000000000000/* Test of gl_thread_self () macro. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include "glthread/thread.h" gl_thread_t main_thread; int main () { /* Check that gl_thread_self () can be used with just $(LIBTHREAD), not $(LIBMULTITHREAD), i.e. in libraries that are multithread-safe but don't create threads themselves. */ main_thread = gl_thread_self (); return 0; } gnuastro-0.5/bootstrapped/tests/test-thread_create.c0000644000175000017500000000412413217200024017714 00000000000000/* Test of gl_thread_create () macro. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include "glthread/thread.h" #include #include #include "macros.h" static gl_thread_t main_thread_before; static gl_thread_t main_thread_after; static gl_thread_t worker_thread; static int dummy; static volatile int work_done; static void * worker_thread_func (void *arg) { work_done = 1; return &dummy; } int main () { main_thread_before = gl_thread_self (); if (glthread_create (&worker_thread, worker_thread_func, NULL) == 0) { void *ret; /* Check that gl_thread_self () has the same value before than after the first call to gl_thread_create (). */ main_thread_after = gl_thread_self (); ASSERT (memcmp (&main_thread_before, &main_thread_after, sizeof (gl_thread_t)) == 0); gl_thread_join (worker_thread, &ret); /* Check the return value of the thread. */ ASSERT (ret == &dummy); /* Check that worker_thread_func () has finished executing. */ ASSERT (work_done); return 0; } else { #if USE_POSIX_THREADS || USE_SOLARIS_THREADS || USE_PTH_THREADS || USE_WINDOWS_THREADS fputs ("glthread_create failed\n", stderr); return 1; #else fputs ("Skipping test: multithreading not enabled\n", stderr); return 77; #endif } } gnuastro-0.5/bootstrapped/tests/test-sysexits.c0000644000175000017500000000255213217200024017020 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include int exitcode; int main () { /* Check that all EX_* symbols are defined to integer constant expressions with mutually different values. */ switch (exitcode) { case EX_OK: case EX_USAGE: case EX_DATAERR: case EX_NOINPUT: case EX_NOUSER: case EX_NOHOST: case EX_UNAVAILABLE: case EX_SOFTWARE: case EX_OSERR: case EX_OSFILE: case EX_CANTCREAT: case EX_IOERR: case EX_TEMPFAIL: case EX_PROTOCOL: case EX_NOPERM: case EX_CONFIG: break; } return 0; } gnuastro-0.5/bootstrapped/tests/test-sys_uio.c0000644000175000017500000000173613217200024016622 00000000000000/* Test of substitute. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2011. */ #include #include /* Check that necessary types are defined. */ size_t a; ssize_t b; struct iovec c; int main (void) { return a + b + !!c.iov_base + c.iov_len; } gnuastro-0.5/bootstrapped/tests/test-sys_types.c0000644000175000017500000000172213217200024017165 00000000000000/* Test of substitute. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include /* Check that the types are all defined. */ pid_t t1; size_t t2; ssize_t t3; off_t t4; mode_t t5; int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-sys_time.c0000644000175000017500000000215013217200024016753 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include /* Check that the 'struct timeval' type is defined. */ struct timeval a; /* Check that a.tv_sec is wide enough to hold a time_t, ignoring signedness issues. */ typedef int verify_tv_sec_type[sizeof (time_t) <= sizeof (a.tv_sec) ? 1 : -1]; int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-sys_stat.c0000644000175000017500000001626613217200024017005 00000000000000/* Test of substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check the existence of some macros. */ int a[] = { S_IFMT, #ifdef S_IFBLK /* missing on MSVC */ S_IFBLK, #endif S_IFCHR, S_IFDIR, S_IFIFO, S_IFREG, #ifdef S_IFLNK /* missing on native Windows and DJGPP */ S_IFLNK, #endif #ifdef S_IFSOCK /* missing on native Windows and DJGPP */ S_IFSOCK, #endif S_IRWXU, S_IRUSR, S_IWUSR, S_IXUSR, S_IRWXG, S_IRGRP, S_IWGRP, S_IXGRP, S_IRWXO, S_IROTH, S_IWOTH, S_IXOTH, S_ISUID, S_ISGID, S_ISVTX, S_ISBLK (S_IFREG), S_ISCHR (S_IFREG), S_ISDIR (S_IFREG), S_ISFIFO (S_IFREG), S_ISREG (S_IFREG), S_ISLNK (S_IFREG), S_ISSOCK (S_IFREG), S_ISDOOR (S_IFREG), S_ISMPB (S_IFREG), S_ISMPX (S_IFREG), S_ISNAM (S_IFREG), S_ISNWK (S_IFREG), S_ISPORT (S_IFREG), S_ISCTG (S_IFREG), S_ISOFD (S_IFREG), S_ISOFL (S_IFREG), S_ISWHT (S_IFREG) }; /* Sanity checks. */ verify (S_IRWXU == (S_IRUSR | S_IWUSR | S_IXUSR)); verify (S_IRWXG == (S_IRGRP | S_IWGRP | S_IXGRP)); verify (S_IRWXO == (S_IROTH | S_IWOTH | S_IXOTH)); #ifdef S_IFBLK verify (S_ISBLK (S_IFBLK)); #endif verify (!S_ISBLK (S_IFCHR)); verify (!S_ISBLK (S_IFDIR)); verify (!S_ISBLK (S_IFIFO)); verify (!S_ISBLK (S_IFREG)); #ifdef S_IFLNK verify (!S_ISBLK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISBLK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISCHR (S_IFBLK)); #endif verify (S_ISCHR (S_IFCHR)); verify (!S_ISCHR (S_IFDIR)); verify (!S_ISCHR (S_IFIFO)); verify (!S_ISCHR (S_IFREG)); #ifdef S_IFLNK verify (!S_ISCHR (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISCHR (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISDIR (S_IFBLK)); #endif verify (!S_ISDIR (S_IFCHR)); verify (S_ISDIR (S_IFDIR)); verify (!S_ISDIR (S_IFIFO)); verify (!S_ISDIR (S_IFREG)); #ifdef S_IFLNK verify (!S_ISDIR (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISDIR (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISFIFO (S_IFBLK)); #endif verify (!S_ISFIFO (S_IFCHR)); verify (!S_ISFIFO (S_IFDIR)); verify (S_ISFIFO (S_IFIFO)); verify (!S_ISFIFO (S_IFREG)); #ifdef S_IFLNK verify (!S_ISFIFO (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISFIFO (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISREG (S_IFBLK)); #endif verify (!S_ISREG (S_IFCHR)); verify (!S_ISREG (S_IFDIR)); verify (!S_ISREG (S_IFIFO)); verify (S_ISREG (S_IFREG)); #ifdef S_IFLNK verify (!S_ISREG (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISREG (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISLNK (S_IFBLK)); #endif verify (!S_ISLNK (S_IFCHR)); verify (!S_ISLNK (S_IFDIR)); verify (!S_ISLNK (S_IFIFO)); verify (!S_ISLNK (S_IFREG)); #ifdef S_IFLNK verify (S_ISLNK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISLNK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISSOCK (S_IFBLK)); #endif verify (!S_ISSOCK (S_IFCHR)); verify (!S_ISSOCK (S_IFDIR)); verify (!S_ISSOCK (S_IFIFO)); verify (!S_ISSOCK (S_IFREG)); #ifdef S_IFLNK verify (!S_ISSOCK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (S_ISSOCK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISDOOR (S_IFBLK)); #endif verify (!S_ISDOOR (S_IFCHR)); verify (!S_ISDOOR (S_IFDIR)); verify (!S_ISDOOR (S_IFIFO)); verify (!S_ISDOOR (S_IFREG)); #ifdef S_IFLNK verify (!S_ISDOOR (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISDOOR (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISMPB (S_IFBLK)); #endif verify (!S_ISMPB (S_IFCHR)); verify (!S_ISMPB (S_IFDIR)); verify (!S_ISMPB (S_IFIFO)); verify (!S_ISMPB (S_IFREG)); #ifdef S_IFLNK verify (!S_ISMPB (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISMPB (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISMPX (S_IFBLK)); #endif verify (!S_ISMPX (S_IFCHR)); verify (!S_ISMPX (S_IFDIR)); verify (!S_ISMPX (S_IFIFO)); verify (!S_ISMPX (S_IFREG)); #ifdef S_IFLNK verify (!S_ISMPX (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISMPX (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISNAM (S_IFBLK)); #endif verify (!S_ISNAM (S_IFCHR)); verify (!S_ISNAM (S_IFDIR)); verify (!S_ISNAM (S_IFIFO)); verify (!S_ISNAM (S_IFREG)); #ifdef S_IFLNK verify (!S_ISNAM (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISNAM (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISNWK (S_IFBLK)); #endif verify (!S_ISNWK (S_IFCHR)); verify (!S_ISNWK (S_IFDIR)); verify (!S_ISNWK (S_IFIFO)); verify (!S_ISNWK (S_IFREG)); #ifdef S_IFLNK verify (!S_ISNWK (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISNWK (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISPORT (S_IFBLK)); #endif verify (!S_ISPORT (S_IFCHR)); verify (!S_ISPORT (S_IFDIR)); verify (!S_ISPORT (S_IFIFO)); verify (!S_ISPORT (S_IFREG)); #ifdef S_IFLNK verify (!S_ISPORT (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISPORT (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISCTG (S_IFBLK)); #endif verify (!S_ISCTG (S_IFCHR)); verify (!S_ISCTG (S_IFDIR)); verify (!S_ISCTG (S_IFIFO)); verify (!S_ISCTG (S_IFREG)); #ifdef S_IFLNK verify (!S_ISCTG (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISCTG (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISOFD (S_IFBLK)); #endif verify (!S_ISOFD (S_IFCHR)); verify (!S_ISOFD (S_IFDIR)); verify (!S_ISOFD (S_IFIFO)); verify (!S_ISOFD (S_IFREG)); #ifdef S_IFLNK verify (!S_ISOFD (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISOFD (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISOFL (S_IFBLK)); #endif verify (!S_ISOFL (S_IFCHR)); verify (!S_ISOFL (S_IFDIR)); verify (!S_ISOFL (S_IFIFO)); verify (!S_ISOFL (S_IFREG)); #ifdef S_IFLNK verify (!S_ISOFL (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISOFL (S_IFSOCK)); #endif #ifdef S_IFBLK verify (!S_ISWHT (S_IFBLK)); #endif verify (!S_ISWHT (S_IFCHR)); verify (!S_ISWHT (S_IFDIR)); verify (!S_ISWHT (S_IFIFO)); verify (!S_ISWHT (S_IFREG)); #ifdef S_IFLNK verify (!S_ISWHT (S_IFLNK)); #endif #ifdef S_IFSOCK verify (!S_ISWHT (S_IFSOCK)); #endif /* POSIX 2008 requires traditional encoding of permission constants. */ verify (S_IRWXU == 00700); verify (S_IRUSR == 00400); verify (S_IWUSR == 00200); verify (S_IXUSR == 00100); verify (S_IRWXG == 00070); verify (S_IRGRP == 00040); verify (S_IWGRP == 00020); verify (S_IXGRP == 00010); verify (S_IRWXO == 00007); verify (S_IROTH == 00004); verify (S_IWOTH == 00002); verify (S_IXOTH == 00001); verify (S_ISUID == 04000); verify (S_ISGID == 02000); verify (S_ISVTX == 01000); #if ((0 <= UTIME_NOW && UTIME_NOW < 1000000000) \ || (0 <= UTIME_OMIT && UTIME_OMIT < 1000000000) \ || UTIME_NOW == UTIME_OMIT) invalid UTIME macros #endif /* Check the existence of some types. */ nlink_t t1; off_t t2; mode_t t3; struct timespec st; int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-sys_socket.c0000644000175000017500000000330113217200024017304 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include #if HAVE_SHUTDOWN /* Check some integer constant expressions. */ int a[] = { SHUT_RD, SHUT_WR, SHUT_RDWR }; #endif /* Check that the 'socklen_t' type is defined. */ socklen_t t1; /* Check that the 'size_t' and 'ssize_t' types are defined. */ size_t t2; ssize_t t3; /* Check that 'struct iovec' is defined. */ struct iovec io; /* Check that a minimal set of 'struct msghdr' is defined. */ struct msghdr msg; int main (void) { struct sockaddr_storage x; sa_family_t i; /* Check some errno values. */ switch (ENOTSOCK) { case ENOTSOCK: case EADDRINUSE: case ENETRESET: case ECONNABORTED: case ECONNRESET: case ENOTCONN: case ESHUTDOWN: break; } x.ss_family = 42; i = 42; msg.msg_iov = &io; return (x.ss_family - i + msg.msg_namelen + msg.msg_iov->iov_len + msg.msg_iovlen); } gnuastro-0.5/bootstrapped/tests/test-sys_select.c0000644000175000017500000000336213217200024017302 00000000000000/* Test of substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" /* The following may be macros without underlying functions, so only check signature if they are not macros. */ #ifndef FD_CLR SIGNATURE_CHECK (FD_CLR, void, (int, fd_set *)); #endif #ifndef FD_ISSET SIGNATURE_CHECK (FD_ISSET, void, (int, fd_set *)); #endif #ifndef FD_SET SIGNATURE_CHECK (FD_SET, int, (int, fd_set *)); #endif #ifndef FD_ZERO SIGNATURE_CHECK (FD_ZERO, void, (fd_set *)); #endif /* Check that the 'struct timeval' type is defined. */ struct timeval a; /* Check that a.tv_sec is wide enough to hold a time_t, ignoring signedness issues. */ typedef int verify_tv_sec_type[sizeof (time_t) <= sizeof (a.tv_sec) ? 1 : -1]; /* Check that sigset_t is defined. */ sigset_t t2; int main (void) { /* Check that FD_ZERO can be used. This should not yield a warning such as "warning: implicit declaration of function 'memset'". */ fd_set fds; FD_ZERO (&fds); return 0; } gnuastro-0.5/bootstrapped/tests/test-sys_ioctl.c0000644000175000017500000000155113217200024017133 00000000000000/* Test of substitute. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-symlink.c0000644000175000017500000000242313217200024016610 00000000000000/* Tests of symlink. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (symlink, int, (char const *, char const *)); #include #include #include #include #include #include #include "ignore-value.h" #include "macros.h" #define BASE "test-symlink.t" #include "test-symlink.h" int main (void) { /* Remove any leftovers from a previous partial run. */ ignore_value (system ("rm -rf " BASE "*")); return test_symlink (symlink, true); } gnuastro-0.5/bootstrapped/tests/test-strtod.c0000644000175000017500000007053113217200024016446 00000000000000/* * Copyright (C) 2008-2017 Free Software Foundation, Inc. * Written by Eric Blake * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (strtod, double, (char const *, char **)); #include #include #include #include #include "isnand-nolibm.h" #include "minus-zero.h" #include "macros.h" /* Avoid requiring -lm just for fabs. */ #define FABS(d) ((d) < 0.0 ? -(d) : (d)) int main (void) { int status = 0; /* Subject sequence empty or invalid. */ { const char input[] = ""; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " "; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " +"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " ."; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " .e0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); /* IRIX 6.5, OSF/1 5.1 */ ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " +.e-0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); /* IRIX 6.5, OSF/1 5.1 */ ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " in"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); } { const char input[] = " na"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); } /* Simple floating point values. */ { const char input[] = "1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = "1."; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = ".5"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); /* FIXME - gnulib's version is rather inaccurate. It would be nice to guarantee an exact result, but for now, we settle for a 1-ulp error. */ ASSERT (FABS (result - 0.5) < DBL_EPSILON); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = " 1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = "+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = "-1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == -1.0); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = "1e0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 3); ASSERT (errno == 0); } { const char input[] = "1e+0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 4); ASSERT (errno == 0); } { const char input[] = "1e-0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 4); ASSERT (errno == 0); } { const char input[] = "1e1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 10.0); ASSERT (ptr == input + 3); ASSERT (errno == 0); } { const char input[] = "5e-1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); /* FIXME - gnulib's version is rather inaccurate. It would be nice to guarantee an exact result, but for now, we settle for a 1-ulp error. */ ASSERT (FABS (result - 0.5) < DBL_EPSILON); ASSERT (ptr == input + 4); ASSERT (errno == 0); } /* Zero. */ { const char input[] = "0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = ".0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = "0e0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 3); ASSERT (errno == 0); } { const char input[] = "0e+9999999"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 10); ASSERT (errno == 0); } { const char input[] = "0e-9999999"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 10); ASSERT (errno == 0); } { const char input[] = "-0"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!!signbit (result) == !!signbit (minus_zerod)); /* IRIX 6.5, OSF/1 4.0 */ ASSERT (ptr == input + 2); ASSERT (errno == 0); } /* Suffixes. */ { const char input[] = "1f"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = "1.f"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = "1e"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = "1e+"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = "1e-"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = "1E 2"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* HP-UX 11.11, IRIX 6.5, OSF/1 4.0 */ ASSERT (ptr == input + 1); /* HP-UX 11.11, IRIX 6.5 */ ASSERT (errno == 0); } { const char input[] = "0x"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "00x1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 2); ASSERT (errno == 0); } { const char input[] = "-0x"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!!signbit (result) == !!signbit (minus_zerod)); /* Mac OS X 10.3, FreeBSD 6.2, IRIX 6.5, OSF/1 4.0 */ ASSERT (ptr == input + 2); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0xg"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0xp"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0XP"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0x."; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0xp+"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0xp+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "0x.p+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input + 1); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, AIX 7.1 */ ASSERT (errno == 0); } { const char input[] = "1p+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } { const char input[] = "1P+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + 1); ASSERT (errno == 0); } /* Overflow/underflow. */ { const char input[] = "1E1000000"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == HUGE_VAL); ASSERT (ptr == input + 9); /* OSF/1 5.1 */ ASSERT (errno == ERANGE); } { const char input[] = "-1E1000000"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == -HUGE_VAL); ASSERT (ptr == input + 10); ASSERT (errno == ERANGE); } { const char input[] = "1E-100000"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (0.0 <= result && result <= DBL_MIN); ASSERT (!signbit (result)); ASSERT (ptr == input + 9); ASSERT (errno == ERANGE); } { const char input[] = "-1E-100000"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (-DBL_MIN <= result && result <= 0.0); #if 0 /* FIXME - this is glibc bug 5995; POSIX allows returning positive 0 on negative underflow, even though quality of implementation demands preserving the sign. Disable this test until fixed glibc is more prevalent. */ ASSERT (!!signbit (result) == !!signbit (minus_zerod)); /* glibc-2.3.6, mingw */ #endif ASSERT (ptr == input + 10); ASSERT (errno == ERANGE); } { const char input[] = "1E 1000000"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* HP-UX 11.11, IRIX 6.5, OSF/1 4.0 */ ASSERT (ptr == input + 1); /* HP-UX 11.11, IRIX 6.5 */ ASSERT (errno == 0); } { const char input[] = "0x1P 1000000"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } /* Infinity. */ { const char input[] = "iNf"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == HUGE_VAL); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + 3); /* OpenBSD 4.0, HP-UX 11.00, IRIX 6.5, OSF/1 5.1, Solaris 9, mingw */ ASSERT (errno == 0); /* HP-UX 11.11, OSF/1 4.0 */ } { const char input[] = "-InF"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == -HUGE_VAL); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + 4); /* OpenBSD 4.0, HP-UX 11.00, IRIX 6.5, OSF/1 4.0, Solaris 9, mingw */ ASSERT (errno == 0); /* HP-UX 11.11, OSF/1 4.0 */ } { const char input[] = "infinite"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == HUGE_VAL); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + 3); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (errno == 0); /* OSF/1 4.0 */ } { const char input[] = "infinitY"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == HUGE_VAL); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + 8); /* OpenBSD 4.0, HP-UX 11.00, IRIX 6.5, OSF/1 5.1, Solaris 9, mingw */ ASSERT (errno == 0); /* HP-UX 11.11, OSF/1 4.0 */ } { const char input[] = "infinitY."; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == HUGE_VAL); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + 8); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (errno == 0); /* OSF/1 4.0 */ } /* NaN. Some processors set the sign bit of the default NaN, so all we check is that using a sign changes the result. */ { const char input[] = "-nan"; char *ptr1; char *ptr2; double result1; double result2; errno = 0; result1 = strtod (input, &ptr1); result2 = strtod (input + 1, &ptr2); #if 1 /* All known CPUs support NaNs. */ ASSERT (isnand (result1)); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (isnand (result2)); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ # if 0 /* Sign bits of NaN is a portability sticking point, not worth worrying about. */ ASSERT (!!signbit (result1) != !!signbit (result2)); /* glibc-2.3.6, IRIX 6.5, OSF/1 5.1, mingw */ # endif ASSERT (ptr1 == input + 4); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, Solaris 2.5.1, mingw */ ASSERT (ptr2 == input + 4); /* OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, Solaris 2.5.1, mingw */ ASSERT (errno == 0); /* HP-UX 11.11 */ #else ASSERT (result1 == 0.0); ASSERT (result2 == 0.0); ASSERT (!signbit (result1)); ASSERT (!signbit (result2)); ASSERT (ptr1 == input); ASSERT (ptr2 == input + 1); ASSERT (errno == 0 || errno == EINVAL); #endif } { const char input[] = "+nan("; char *ptr1; char *ptr2; double result1; double result2; errno = 0; result1 = strtod (input, &ptr1); result2 = strtod (input + 1, &ptr2); #if 1 /* All known CPUs support NaNs. */ ASSERT (isnand (result1)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (isnand (result2)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (!!signbit (result1) == !!signbit (result2)); ASSERT (ptr1 == input + 4); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 2.5.1, mingw */ ASSERT (ptr2 == input + 4); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 2.5.1, mingw */ ASSERT (errno == 0); #else ASSERT (result1 == 0.0); ASSERT (result2 == 0.0); ASSERT (!signbit (result1)); ASSERT (!signbit (result2)); ASSERT (ptr1 == input); ASSERT (ptr2 == input + 1); ASSERT (errno == 0 || errno == EINVAL); #endif } { const char input[] = "-nan()"; char *ptr1; char *ptr2; double result1; double result2; errno = 0; result1 = strtod (input, &ptr1); result2 = strtod (input + 1, &ptr2); #if 1 /* All known CPUs support NaNs. */ ASSERT (isnand (result1)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (isnand (result2)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ # if 0 /* Sign bits of NaN is a portability sticking point, not worth worrying about. */ ASSERT (!!signbit (result1) != !!signbit (result2)); /* glibc-2.3.6, IRIX 6.5, OSF/1 5.1, mingw */ # endif ASSERT (ptr1 == input + 6); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr2 == input + 6); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (errno == 0); #else ASSERT (result1 == 0.0); ASSERT (result2 == 0.0); ASSERT (!signbit (result1)); ASSERT (!signbit (result2)); ASSERT (ptr1 == input); ASSERT (ptr2 == input + 1); ASSERT (errno == 0 || errno == EINVAL); #endif } { const char input[] = " nan()."; char *ptr; double result; errno = 0; result = strtod (input, &ptr); #if 1 /* All known CPUs support NaNs. */ ASSERT (isnand (result)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + 6); /* glibc-2.3.6, Mac OS X 10.3, FreeBSD 6.2, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (errno == 0); #else ASSERT (result == 0.0); ASSERT (!signbit (result)); ASSERT (ptr == input); ASSERT (errno == 0 || errno == EINVAL); #endif } { /* The behavior of nan(0) is implementation-defined, but all implementations we know of which handle optional n-char-sequences handle nan(0) the same as nan(). */ const char input[] = "-nan(0)."; char *ptr1; char *ptr2; double result1; double result2; errno = 0; result1 = strtod (input, &ptr1); result2 = strtod (input + 1, &ptr2); #if 1 /* All known CPUs support NaNs. */ ASSERT (isnand (result1)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (isnand (result2)); /* OpenBSD 4.0, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ # if 0 /* Sign bits of NaN is a portability sticking point, not worth worrying about. */ ASSERT (!!signbit (result1) != !!signbit (result2)); /* glibc-2.3.6, IRIX 6.5, OSF/1 5.1, mingw */ # endif ASSERT (ptr1 == input + 7); /* glibc-2.3.6, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr2 == input + 7); /* glibc-2.3.6, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (errno == 0); #else ASSERT (result1 == 0.0); ASSERT (result2 == 0.0); ASSERT (!signbit (result1)); ASSERT (!signbit (result2)); ASSERT (ptr1 == input); ASSERT (ptr2 == input + 1); ASSERT (errno == 0 || errno == EINVAL); #endif } /* Hex. */ { const char input[] = "0xa"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 10.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0XA"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 10.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0x1p"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0x1p+"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0x1P+"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0x1p+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 2.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 6); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0X1P+1"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 2.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 6); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0x1p+1a"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 2.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 6); /* NetBSD 3.0, OpenBSD 4.0, AIX 5.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } { const char input[] = "0x1p 2"; char *ptr; double result; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* NetBSD 3.0, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (ptr == input + 3); /* NetBSD 3.0, OpenBSD 4.0, AIX 7.1, HP-UX 11.11, IRIX 6.5, OSF/1 5.1, Solaris 10, mingw */ ASSERT (errno == 0); } /* Large buffers. */ { size_t m = 1000000; char *input = malloc (m + 1); if (input) { char *ptr; double result; memset (input, '\t', m - 1); input[m - 1] = '1'; input[m] = '\0'; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + m); ASSERT (errno == 0); } free (input); } { size_t m = 1000000; char *input = malloc (m + 1); if (input) { char *ptr; double result; memset (input, '0', m - 1); input[m - 1] = '1'; input[m] = '\0'; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); ASSERT (ptr == input + m); ASSERT (errno == 0); } free (input); } #if 0 /* Newlib has an artificial limit of 20000 for the exponent. TODO - gnulib should fix this. */ { size_t m = 1000000; char *input = malloc (m + 1); if (input) { char *ptr; double result; input[0] = '.'; memset (input + 1, '0', m - 10); input[m - 9] = '1'; input[m - 8] = 'e'; input[m - 7] = '+'; input[m - 6] = '9'; input[m - 5] = '9'; input[m - 4] = '9'; input[m - 3] = '9'; input[m - 2] = '9'; input[m - 1] = '1'; input[m] = '\0'; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* Mac OS X 10.3, FreeBSD 6.2, NetBSD 3.0, OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + m); /* OSF/1 5.1 */ ASSERT (errno == 0); /* Mac OS X 10.3, FreeBSD 6.2, NetBSD 3.0, OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ } free (input); } { size_t m = 1000000; char *input = malloc (m + 1); if (input) { char *ptr; double result; input[0] = '1'; memset (input + 1, '0', m - 9); input[m - 8] = 'e'; input[m - 7] = '-'; input[m - 6] = '9'; input[m - 5] = '9'; input[m - 4] = '9'; input[m - 3] = '9'; input[m - 2] = '9'; input[m - 1] = '1'; input[m] = '\0'; errno = 0; result = strtod (input, &ptr); ASSERT (result == 1.0); /* Mac OS X 10.3, FreeBSD 6.2, NetBSD 3.0, OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ ASSERT (ptr == input + m); ASSERT (errno == 0); /* Mac OS X 10.3, FreeBSD 6.2, NetBSD 3.0, OpenBSD 4.0, IRIX 6.5, OSF/1 5.1, mingw */ } free (input); } #endif { size_t m = 1000000; char *input = malloc (m + 1); if (input) { char *ptr; double result; input[0] = '-'; input[1] = '0'; input[2] = 'e'; input[3] = '1'; memset (input + 4, '0', m - 3); input[m] = '\0'; errno = 0; result = strtod (input, &ptr); ASSERT (result == 0.0); ASSERT (!!signbit (result) == !!signbit (minus_zerod)); /* IRIX 6.5, OSF/1 4.0 */ ASSERT (ptr == input + m); ASSERT (errno == 0); } free (input); } /* Rounding. */ /* TODO - is it worth some tests of rounding for typical IEEE corner cases, such as .5 ULP rounding up to the smallest denormal and not causing underflow, or DBL_MIN - .5 ULP not causing an infinite loop? */ return status; } gnuastro-0.5/bootstrapped/tests/test-strnlen.c0000644000175000017500000000336213217200024016612 00000000000000/* * Copyright (C) 2010-2017 Free Software Foundation, Inc. * Written by Eric Blake * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (strnlen, size_t, (char const *, size_t)); #include #include "zerosize-ptr.h" #include "macros.h" int main (void) { size_t i; char *page_boundary = (char *) zerosize_ptr (); if (!page_boundary) { page_boundary = malloc (0x1000); ASSERT (page_boundary); page_boundary += 0x1000; } /* Basic behavior tests. */ ASSERT (strnlen ("a", 0) == 0); ASSERT (strnlen ("a", 1) == 1); ASSERT (strnlen ("a", 2) == 1); ASSERT (strnlen ("", 0x100000) == 0); /* Memory fence and alignment testing. */ for (i = 0; i < 512; i++) { char *start = page_boundary - i; size_t j = i; memset (start, 'x', i); do { if (i != j) { start[j] = 0; ASSERT (strnlen (start, i + j) == j); } ASSERT (strnlen (start, i) == j); ASSERT (strnlen (start, j) == j); } while (j--); } return 0; } gnuastro-0.5/bootstrapped/tests/test-strings.c0000644000175000017500000000155413217200024016617 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include int main () { return 0; } gnuastro-0.5/bootstrapped/tests/test-string.c0000644000175000017500000000201013217200024016420 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-strerror_r.c0000644000175000017500000001172713217200024017334 00000000000000/* Test of strerror_r() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (strerror_r, int, (int, char *, size_t)); #include #include "macros.h" int main (void) { char buf[100]; int ret; /* Test results with valid errnum and enough room. */ errno = 0; buf[0] = '\0'; ASSERT (strerror_r (EACCES, buf, sizeof buf) == 0); ASSERT (buf[0] != '\0'); ASSERT (errno == 0); ASSERT (strlen (buf) < sizeof buf); errno = 0; buf[0] = '\0'; ASSERT (strerror_r (ETIMEDOUT, buf, sizeof buf) == 0); ASSERT (buf[0] != '\0'); ASSERT (errno == 0); ASSERT (strlen (buf) < sizeof buf); errno = 0; buf[0] = '\0'; ASSERT (strerror_r (EOVERFLOW, buf, sizeof buf) == 0); ASSERT (buf[0] != '\0'); ASSERT (errno == 0); ASSERT (strlen (buf) < sizeof buf); /* POSIX requires strerror (0) to succeed. Reject use of "Unknown error", but allow "Success", "No error", or even Solaris' "Error 0" which are distinct patterns from true out-of-range strings. http://austingroupbugs.net/view.php?id=382 */ errno = 0; buf[0] = '\0'; ret = strerror_r (0, buf, sizeof buf); ASSERT (ret == 0); ASSERT (buf[0]); ASSERT (errno == 0); ASSERT (strstr (buf, "nknown") == NULL); ASSERT (strstr (buf, "ndefined") == NULL); /* Test results with out-of-range errnum and enough room. POSIX allows an empty string on success, and allows an unchanged buf on error, but these are not useful, so we guarantee contents. */ errno = 0; buf[0] = '^'; ret = strerror_r (-3, buf, sizeof buf); ASSERT (ret == 0 || ret == EINVAL); ASSERT (buf[0] != '^'); ASSERT (*buf); ASSERT (errno == 0); ASSERT (strlen (buf) < sizeof buf); /* Test results with a too small buffer. POSIX requires an error; only ERANGE for 0 and valid errors, and a choice of ERANGE or EINVAL for out-of-range values. On error, POSIX permits buf to be empty, unchanged, or unterminated, but these are not useful, so we guarantee NUL-terminated truncated contents for all but size 0. http://austingroupbugs.net/view.php?id=398. Also ensure that no out-of-bounds writes occur. */ { int errs[] = { EACCES, 0, -3, }; int j; buf[sizeof buf - 1] = '\0'; for (j = 0; j < SIZEOF (errs); j++) { int err = errs[j]; char buf2[sizeof buf] = ""; size_t len; size_t i; strerror_r (err, buf2, sizeof buf2); len = strlen (buf2); ASSERT (len < sizeof buf); for (i = 0; i <= len; i++) { memset (buf, '^', sizeof buf - 1); errno = 0; ret = strerror_r (err, buf, i); ASSERT (errno == 0); if (j == 2) ASSERT (ret == ERANGE || ret == EINVAL); else ASSERT (ret == ERANGE); if (i) { ASSERT (strncmp (buf, buf2, i - 1) == 0); ASSERT (buf[i - 1] == '\0'); } ASSERT (strspn (buf + i, "^") == sizeof buf - 1 - i); } strcpy (buf, "BADFACE"); errno = 0; ret = strerror_r (err, buf, len + 1); ASSERT (ret != ERANGE); ASSERT (errno == 0); ASSERT (strcmp (buf, buf2) == 0); } } #if GNULIB_STRERROR /* Test that strerror_r does not clobber strerror buffer. On some platforms, this test can only succeed if gnulib also replaces strerror. */ { const char *msg1; const char *msg2; const char *msg3; const char *msg4; char *str1; char *str2; char *str3; char *str4; msg1 = strerror (ENOENT); ASSERT (msg1); str1 = strdup (msg1); ASSERT (str1); msg2 = strerror (ERANGE); ASSERT (msg2); str2 = strdup (msg2); ASSERT (str2); msg3 = strerror (-4); ASSERT (msg3); str3 = strdup (msg3); ASSERT (str3); msg4 = strerror (1729576); ASSERT (msg4); str4 = strdup (msg4); ASSERT (str4); strerror_r (EACCES, buf, sizeof buf); strerror_r (-5, buf, sizeof buf); ASSERT (msg1 == msg2 || msg1 == msg4 || STREQ (msg1, str1)); ASSERT (msg2 == msg4 || STREQ (msg2, str2)); ASSERT (msg3 == msg4 || STREQ (msg3, str3)); ASSERT (STREQ (msg4, str4)); free (str1); free (str2); free (str3); free (str4); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-strerror.c0000644000175000017500000000371013217200024017004 00000000000000/* Test of strerror() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (strerror, char *, (int)); #include #include "macros.h" int main (void) { char *str; errno = 0; str = strerror (EACCES); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); errno = 0; str = strerror (ETIMEDOUT); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); errno = 0; str = strerror (EOVERFLOW); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); /* POSIX requires strerror (0) to succeed. Reject use of "Unknown error", but allow "Success", "No error", or even Solaris' "Error 0" which are distinct patterns from true out-of-range strings. http://austingroupbugs.net/view.php?id=382 */ errno = 0; str = strerror (0); ASSERT (str); ASSERT (*str); ASSERT (errno == 0); ASSERT (strstr (str, "nknown") == NULL); ASSERT (strstr (str, "ndefined") == NULL); /* POSIX requires strerror to produce a non-NULL result for all inputs; as an extension, we also guarantee a non-empty result. Reporting EINVAL is optional. */ errno = 0; str = strerror (-3); ASSERT (str); ASSERT (*str); ASSERT (errno == 0 || errno == EINVAL); return 0; } gnuastro-0.5/bootstrapped/tests/test-strchrnul.c0000644000175000017500000000444713217200024017156 00000000000000/* * Copyright (C) 2008-2017 Free Software Foundation, Inc. * Written by Eric Blake and Bruno Haible * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (strchrnul, char *, (char const *, int)); #include #include "macros.h" int main (void) { size_t n = 0x100000; char *input = malloc (n + 1); ASSERT (input); input[0] = 'a'; input[1] = 'b'; memset (input + 2, 'c', 1024); memset (input + 1026, 'd', n - 1028); input[n - 2] = 'e'; input[n - 1] = 'a'; input[n] = '\0'; /* Basic behavior tests. */ ASSERT (strchrnul (input, 'a') == input); ASSERT (strchrnul (input, 'b') == input + 1); ASSERT (strchrnul (input, 'c') == input + 2); ASSERT (strchrnul (input, 'd') == input + 1026); ASSERT (strchrnul (input + 1, 'a') == input + n - 1); ASSERT (strchrnul (input + 1, 'e') == input + n - 2); ASSERT (strchrnul (input, 'f') == input + n); ASSERT (strchrnul (input, '\0') == input + n); /* Check that a very long haystack is handled quickly if the byte is found near the beginning. */ { size_t repeat = 10000; for (; repeat > 0; repeat--) { ASSERT (strchrnul (input, 'c') == input + 2); } } /* Alignment tests. */ { int i, j; for (i = 0; i < 32; i++) { for (j = 0; j < 256; j++) input[i + j] = (j + 1) & 0xff; for (j = 1; j < 256; j++) { ASSERT (strchrnul (input + i, j) == input + i + j - 1); input[i + j - 1] = (j == 1 ? 2 : 1); ASSERT (strchrnul (input + i, j) == input + i + 255); input[i + j - 1] = j; } } } free (input); return 0; } gnuastro-0.5/bootstrapped/tests/test-stdlib.c0000644000175000017500000000262513217200024016407 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that EXIT_SUCCESS is 0, per POSIX. */ static int exitcode = EXIT_SUCCESS; #if EXIT_SUCCESS "oops" #endif /* Check for GNU value (not guaranteed by POSIX, but is guaranteed by gnulib). */ #if EXIT_FAILURE != 1 "oops" #endif /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); #if GNULIB_TEST_SYSTEM_POSIX # include "test-sys_wait.h" #else # define test_sys_wait_macros() 0 #endif int main (void) { if (test_sys_wait_macros ()) return 1; return exitcode; } gnuastro-0.5/bootstrapped/tests/test-stdio.c0000644000175000017500000000232313217200024016243 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" /* Check that the various SEEK_* macros are defined. */ int sk[] = { SEEK_CUR, SEEK_END, SEEK_SET }; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); /* Check that the types are all defined. */ fpos_t t1; off_t t2; size_t t3; ssize_t t4; va_list t5; int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-stdint.c0000644000175000017500000003330613217200024016433 00000000000000/* Test of substitute. Copyright (C) 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2006. */ #include /* Whether to enable pedantic checks. */ #define DO_PEDANTIC 0 #include #include "verify.h" #include "intprops.h" #if __GNUC__ >= 2 && DO_PEDANTIC # define verify_same_types(expr1,expr2) \ extern void _verify_func(__LINE__) (__typeof__ (expr1) *); \ extern void _verify_func(__LINE__) (__typeof__ (expr2) *); # define _verify_func(line) _verify_func2(line) # define _verify_func2(line) verify_func_ ## line #else # define verify_same_types(expr1,expr2) extern void verify_func (int) #endif /* 7.18.1.1. Exact-width integer types */ /* 7.18.2.1. Limits of exact-width integer types */ int8_t a1[3] = { INT8_C (17), INT8_MIN, INT8_MAX }; verify (TYPE_MINIMUM (int8_t) == INT8_MIN); verify (TYPE_MAXIMUM (int8_t) == INT8_MAX); verify_same_types (INT8_MIN, (int8_t) 0 + 0); verify_same_types (INT8_MAX, (int8_t) 0 + 0); int16_t a2[3] = { INT16_C (17), INT16_MIN, INT16_MAX }; verify (TYPE_MINIMUM (int16_t) == INT16_MIN); verify (TYPE_MAXIMUM (int16_t) == INT16_MAX); verify_same_types (INT16_MIN, (int16_t) 0 + 0); verify_same_types (INT16_MAX, (int16_t) 0 + 0); int32_t a3[3] = { INT32_C (17), INT32_MIN, INT32_MAX }; verify (TYPE_MINIMUM (int32_t) == INT32_MIN); verify (TYPE_MAXIMUM (int32_t) == INT32_MAX); verify_same_types (INT32_MIN, (int32_t) 0 + 0); verify_same_types (INT32_MAX, (int32_t) 0 + 0); #ifdef INT64_MAX int64_t a4[3] = { INT64_C (17), INT64_MIN, INT64_MAX }; verify (TYPE_MINIMUM (int64_t) == INT64_MIN); verify (TYPE_MAXIMUM (int64_t) == INT64_MAX); verify_same_types (INT64_MIN, (int64_t) 0 + 0); verify_same_types (INT64_MAX, (int64_t) 0 + 0); #endif uint8_t b1[2] = { UINT8_C (17), UINT8_MAX }; verify (TYPE_MAXIMUM (uint8_t) == UINT8_MAX); verify_same_types (UINT8_MAX, (uint8_t) 0 + 0); uint16_t b2[2] = { UINT16_C (17), UINT16_MAX }; verify (TYPE_MAXIMUM (uint16_t) == UINT16_MAX); verify_same_types (UINT16_MAX, (uint16_t) 0 + 0); uint32_t b3[2] = { UINT32_C (17), UINT32_MAX }; verify (TYPE_MAXIMUM (uint32_t) == UINT32_MAX); verify_same_types (UINT32_MAX, (uint32_t) 0 + 0); #ifdef UINT64_MAX uint64_t b4[2] = { UINT64_C (17), UINT64_MAX }; verify (TYPE_MAXIMUM (uint64_t) == UINT64_MAX); verify_same_types (UINT64_MAX, (uint64_t) 0 + 0); #endif #if INT8_MIN && INT8_MAX && INT16_MIN && INT16_MAX && INT32_MIN && INT32_MAX /* ok */ #else err or; #endif #if UINT8_MAX && UINT16_MAX && UINT32_MAX /* ok */ #else err or; #endif /* 7.18.1.2. Minimum-width integer types */ /* 7.18.2.2. Limits of minimum-width integer types */ int_least8_t c1[3] = { 17, INT_LEAST8_MIN, INT_LEAST8_MAX }; verify (TYPE_MINIMUM (int_least8_t) == INT_LEAST8_MIN); verify (TYPE_MAXIMUM (int_least8_t) == INT_LEAST8_MAX); verify_same_types (INT_LEAST8_MIN, (int_least8_t) 0 + 0); verify_same_types (INT_LEAST8_MAX, (int_least8_t) 0 + 0); int_least16_t c2[3] = { 17, INT_LEAST16_MIN, INT_LEAST16_MAX }; verify (TYPE_MINIMUM (int_least16_t) == INT_LEAST16_MIN); verify (TYPE_MAXIMUM (int_least16_t) == INT_LEAST16_MAX); verify_same_types (INT_LEAST16_MIN, (int_least16_t) 0 + 0); verify_same_types (INT_LEAST16_MAX, (int_least16_t) 0 + 0); int_least32_t c3[3] = { 17, INT_LEAST32_MIN, INT_LEAST32_MAX }; verify (TYPE_MINIMUM (int_least32_t) == INT_LEAST32_MIN); verify (TYPE_MAXIMUM (int_least32_t) == INT_LEAST32_MAX); verify_same_types (INT_LEAST32_MIN, (int_least32_t) 0 + 0); verify_same_types (INT_LEAST32_MAX, (int_least32_t) 0 + 0); #ifdef INT_LEAST64_MAX int_least64_t c4[3] = { 17, INT_LEAST64_MIN, INT_LEAST64_MAX }; verify (TYPE_MINIMUM (int_least64_t) == INT_LEAST64_MIN); verify (TYPE_MAXIMUM (int_least64_t) == INT_LEAST64_MAX); verify_same_types (INT_LEAST64_MIN, (int_least64_t) 0 + 0); verify_same_types (INT_LEAST64_MAX, (int_least64_t) 0 + 0); #endif uint_least8_t d1[2] = { 17, UINT_LEAST8_MAX }; verify (TYPE_MAXIMUM (uint_least8_t) == UINT_LEAST8_MAX); verify_same_types (UINT_LEAST8_MAX, (uint_least8_t) 0 + 0); uint_least16_t d2[2] = { 17, UINT_LEAST16_MAX }; verify (TYPE_MAXIMUM (uint_least16_t) == UINT_LEAST16_MAX); verify_same_types (UINT_LEAST16_MAX, (uint_least16_t) 0 + 0); uint_least32_t d3[2] = { 17, UINT_LEAST32_MAX }; verify (TYPE_MAXIMUM (uint_least32_t) == UINT_LEAST32_MAX); verify_same_types (UINT_LEAST32_MAX, (uint_least32_t) 0 + 0); #ifdef UINT_LEAST64_MAX uint_least64_t d4[2] = { 17, UINT_LEAST64_MAX }; verify (TYPE_MAXIMUM (uint_least64_t) == UINT_LEAST64_MAX); verify_same_types (UINT_LEAST64_MAX, (uint_least64_t) 0 + 0); #endif #if INT_LEAST8_MIN && INT_LEAST8_MAX && INT_LEAST16_MIN && INT_LEAST16_MAX && INT_LEAST32_MIN && INT_LEAST32_MAX /* ok */ #else err or; #endif #if UINT_LEAST8_MAX && UINT_LEAST16_MAX && UINT_LEAST32_MAX /* ok */ #else err or; #endif /* 7.18.1.3. Fastest minimum-width integer types */ /* 7.18.2.3. Limits of fastest minimum-width integer types */ int_fast8_t e1[3] = { 17, INT_FAST8_MIN, INT_FAST8_MAX }; verify (TYPE_MINIMUM (int_fast8_t) == INT_FAST8_MIN); verify (TYPE_MAXIMUM (int_fast8_t) == INT_FAST8_MAX); verify_same_types (INT_FAST8_MIN, (int_fast8_t) 0 + 0); verify_same_types (INT_FAST8_MAX, (int_fast8_t) 0 + 0); int_fast16_t e2[3] = { 17, INT_FAST16_MIN, INT_FAST16_MAX }; verify (TYPE_MINIMUM (int_fast16_t) == INT_FAST16_MIN); verify (TYPE_MAXIMUM (int_fast16_t) == INT_FAST16_MAX); verify_same_types (INT_FAST16_MIN, (int_fast16_t) 0 + 0); verify_same_types (INT_FAST16_MAX, (int_fast16_t) 0 + 0); int_fast32_t e3[3] = { 17, INT_FAST32_MIN, INT_FAST32_MAX }; verify (TYPE_MINIMUM (int_fast32_t) == INT_FAST32_MIN); verify (TYPE_MAXIMUM (int_fast32_t) == INT_FAST32_MAX); verify_same_types (INT_FAST32_MIN, (int_fast32_t) 0 + 0); verify_same_types (INT_FAST32_MAX, (int_fast32_t) 0 + 0); #ifdef INT_FAST64_MAX int_fast64_t e4[3] = { 17, INT_FAST64_MIN, INT_FAST64_MAX }; verify (TYPE_MINIMUM (int_fast64_t) == INT_FAST64_MIN); verify (TYPE_MAXIMUM (int_fast64_t) == INT_FAST64_MAX); verify_same_types (INT_FAST64_MIN, (int_fast64_t) 0 + 0); verify_same_types (INT_FAST64_MAX, (int_fast64_t) 0 + 0); #endif uint_fast8_t f1[2] = { 17, UINT_FAST8_MAX }; verify (TYPE_MAXIMUM (uint_fast8_t) == UINT_FAST8_MAX); verify_same_types (UINT_FAST8_MAX, (uint_fast8_t) 0 + 0); uint_fast16_t f2[2] = { 17, UINT_FAST16_MAX }; verify (TYPE_MAXIMUM (uint_fast16_t) == UINT_FAST16_MAX); verify_same_types (UINT_FAST16_MAX, (uint_fast16_t) 0 + 0); uint_fast32_t f3[2] = { 17, UINT_FAST32_MAX }; verify (TYPE_MAXIMUM (uint_fast32_t) == UINT_FAST32_MAX); verify_same_types (UINT_FAST32_MAX, (uint_fast32_t) 0 + 0); #ifdef UINT_FAST64_MAX uint_fast64_t f4[2] = { 17, UINT_FAST64_MAX }; verify (TYPE_MAXIMUM (uint_fast64_t) == UINT_FAST64_MAX); verify_same_types (UINT_FAST64_MAX, (uint_fast64_t) 0 + 0); #endif #if INT_FAST8_MIN && INT_FAST8_MAX && INT_FAST16_MIN && INT_FAST16_MAX && INT_FAST32_MIN && INT_FAST32_MAX /* ok */ #else err or; #endif #if UINT_FAST8_MAX && UINT_FAST16_MAX && UINT_FAST32_MAX /* ok */ #else err or; #endif /* 7.18.1.4. Integer types capable of holding object pointers */ /* 7.18.2.4. Limits of integer types capable of holding object pointers */ intptr_t g[3] = { 17, INTPTR_MIN, INTPTR_MAX }; verify (TYPE_MINIMUM (intptr_t) == INTPTR_MIN); verify (TYPE_MAXIMUM (intptr_t) == INTPTR_MAX); verify_same_types (INTPTR_MIN, (intptr_t) 0 + 0); verify_same_types (INTPTR_MAX, (intptr_t) 0 + 0); uintptr_t h[2] = { 17, UINTPTR_MAX }; verify (TYPE_MAXIMUM (uintptr_t) == UINTPTR_MAX); verify_same_types (UINTPTR_MAX, (uintptr_t) 0 + 0); #if INTPTR_MIN && INTPTR_MAX && UINTPTR_MAX /* ok */ #else err or; #endif /* 7.18.1.5. Greatest-width integer types */ /* 7.18.2.5. Limits of greatest-width integer types */ intmax_t i[3] = { INTMAX_C (17), INTMAX_MIN, INTMAX_MAX }; verify (TYPE_MINIMUM (intmax_t) == INTMAX_MIN); verify (TYPE_MAXIMUM (intmax_t) == INTMAX_MAX); verify_same_types (INTMAX_MIN, (intmax_t) 0 + 0); verify_same_types (INTMAX_MAX, (intmax_t) 0 + 0); uintmax_t j[2] = { UINTMAX_C (17), UINTMAX_MAX }; verify (TYPE_MAXIMUM (uintmax_t) == UINTMAX_MAX); verify_same_types (UINTMAX_MAX, (uintmax_t) 0 + 0); /* As of 2007, Sun C and HP-UX 10.20 cc don't support 'long long' constants in the preprocessor. */ #if !(defined __SUNPRO_C || (defined __hpux && !defined __GNUC__)) #if INTMAX_MIN && INTMAX_MAX && UINTMAX_MAX /* ok */ #else err or; #endif #endif /* 7.18.3. Limits of other integer types */ #include verify (TYPE_MINIMUM (ptrdiff_t) == PTRDIFF_MIN); verify (TYPE_MAXIMUM (ptrdiff_t) == PTRDIFF_MAX); verify_same_types (PTRDIFF_MIN, (ptrdiff_t) 0 + 0); verify_same_types (PTRDIFF_MAX, (ptrdiff_t) 0 + 0); #if PTRDIFF_MIN && PTRDIFF_MAX /* ok */ #else err or; #endif #include verify (TYPE_MINIMUM (sig_atomic_t) == SIG_ATOMIC_MIN); verify (TYPE_MAXIMUM (sig_atomic_t) == SIG_ATOMIC_MAX); verify_same_types (SIG_ATOMIC_MIN, (sig_atomic_t) 0 + 0); verify_same_types (SIG_ATOMIC_MAX, (sig_atomic_t) 0 + 0); #if SIG_ATOMIC_MIN != 17 && SIG_ATOMIC_MAX /* ok */ #else err or; #endif verify (TYPE_MAXIMUM (size_t) == SIZE_MAX); verify_same_types (SIZE_MAX, (size_t) 0 + 0); #if SIZE_MAX /* ok */ #else err or; #endif #if HAVE_WCHAR_T verify (TYPE_MINIMUM (wchar_t) == WCHAR_MIN); verify (TYPE_MAXIMUM (wchar_t) == WCHAR_MAX); verify_same_types (WCHAR_MIN, (wchar_t) 0 + 0); verify_same_types (WCHAR_MAX, (wchar_t) 0 + 0); # if WCHAR_MIN != 17 && WCHAR_MAX /* ok */ # else err or; # endif #endif #if HAVE_WINT_T # include verify (TYPE_MINIMUM (wint_t) == WINT_MIN); verify (TYPE_MAXIMUM (wint_t) == WINT_MAX); verify_same_types (WINT_MIN, (wint_t) 0 + 0); verify_same_types (WINT_MAX, (wint_t) 0 + 0); # if WINT_MIN != 17 && WINT_MAX /* ok */ # else err or; # endif #endif /* 7.18.4. Macros for integer constants */ verify (INT8_C (17) == 17); verify_same_types (INT8_C (17), (int_least8_t)0 + 0); verify (UINT8_C (17) == 17); verify_same_types (UINT8_C (17), (uint_least8_t)0 + 0); verify (INT16_C (17) == 17); verify_same_types (INT16_C (17), (int_least16_t)0 + 0); verify (UINT16_C (17) == 17); verify_same_types (UINT16_C (17), (uint_least16_t)0 + 0); verify (INT32_C (17) == 17); verify_same_types (INT32_C (17), (int_least32_t)0 + 0); verify (UINT32_C (17) == 17); verify_same_types (UINT32_C (17), (uint_least32_t)0 + 0); #ifdef INT64_C verify (INT64_C (17) == 17); verify_same_types (INT64_C (17), (int_least64_t)0 + 0); #endif #ifdef UINT64_C verify (UINT64_C (17) == 17); verify_same_types (UINT64_C (17), (uint_least64_t)0 + 0); #endif verify (INTMAX_C (17) == 17); verify_same_types (INTMAX_C (17), (intmax_t)0 + 0); verify (UINTMAX_C (17) == 17); verify_same_types (UINTMAX_C (17), (uintmax_t)0 + 0); /* Use _GL_VERIFY (with a fixed-length diagnostic string) rather than verify, because the latter would require forming each stringified expression, and many of these would be so long as to trigger a warning/error like this: test-stdint.c:407:1: error: string length '6980' is greater than the \ length '4095' ISO C99 compilers are required to support \ [-Werror=overlength-strings] */ #define verify_width(width, min, max) \ _GL_VERIFY ((max) >> ((width) - 1 - ((min) < 0)) == 1, \ "verify_width check") /* Macros specified by ISO/IEC TS 18661-1:2014. */ #ifdef INT8_MAX verify_width (INT8_WIDTH, INT8_MIN, INT8_MAX); #endif #ifdef UINT8_MAX verify_width (UINT8_WIDTH, 0, UINT8_MAX); #endif #ifdef INT16_MAX verify_width (INT16_WIDTH, INT16_MIN, INT16_MAX); #endif #ifdef UINT16_MAX verify_width (UINT16_WIDTH, 0, UINT16_MAX); #endif #ifdef INT32_MAX verify_width (INT32_WIDTH, INT32_MIN, INT32_MAX); #endif #ifdef UINT32_MAX verify_width (UINT32_WIDTH, 0, UINT32_MAX); #endif #ifdef INT64_MAX verify_width (INT64_WIDTH, INT64_MIN, INT64_MAX); #endif #ifdef UINT64_MAX verify_width (UINT64_WIDTH, 0, UINT64_MAX); #endif verify_width (INT_LEAST8_WIDTH, INT_LEAST8_MIN, INT_LEAST8_MAX); verify_width (UINT_LEAST8_WIDTH, 0, UINT_LEAST8_MAX); verify_width (INT_LEAST16_WIDTH, INT_LEAST16_MIN, INT_LEAST16_MAX); verify_width (UINT_LEAST16_WIDTH, 0, UINT_LEAST16_MAX); verify_width (INT_LEAST32_WIDTH, INT_LEAST32_MIN, INT_LEAST32_MAX); verify_width (UINT_LEAST32_WIDTH, 0, UINT_LEAST32_MAX); verify_width (INT_LEAST64_WIDTH, INT_LEAST64_MIN, INT_LEAST64_MAX); verify_width (UINT_LEAST64_WIDTH, 0, UINT_LEAST64_MAX); verify_width (INT_FAST8_WIDTH, INT_FAST8_MIN, INT_FAST8_MAX); verify_width (UINT_FAST8_WIDTH, 0, UINT_FAST8_MAX); verify_width (INT_FAST16_WIDTH, INT_FAST16_MIN, INT_FAST16_MAX); verify_width (UINT_FAST16_WIDTH, 0, UINT_FAST16_MAX); verify_width (INT_FAST32_WIDTH, INT_FAST32_MIN, INT_FAST32_MAX); verify_width (UINT_FAST32_WIDTH, 0, UINT_FAST32_MAX); verify_width (INT_FAST64_WIDTH, INT_FAST64_MIN, INT_FAST64_MAX); verify_width (UINT_FAST64_WIDTH, 0, UINT_FAST64_MAX); verify_width (INTPTR_WIDTH, INTPTR_MIN, INTPTR_MAX); verify_width (UINTPTR_WIDTH, 0, UINTPTR_MAX); verify_width (INTMAX_WIDTH, INTMAX_MIN, INTMAX_MAX); verify_width (UINTMAX_WIDTH, 0, UINTMAX_MAX); verify_width (PTRDIFF_WIDTH, PTRDIFF_MIN, PTRDIFF_MAX); verify_width (SIZE_WIDTH, 0, SIZE_MAX); verify_width (WCHAR_WIDTH, WCHAR_MIN, WCHAR_MAX); #ifdef WINT_MAX verify_width (WINT_WIDTH, WINT_MIN, WINT_MAX); #endif #ifdef SIG_ATOMIC_MAX verify_width (SIG_ATOMIC_WIDTH, SIG_ATOMIC_MIN, SIG_ATOMIC_MAX); #endif int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-stddef.c0000644000175000017500000000540013217200024016371 00000000000000/* Test of substitute. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include #include #include "verify.h" /* Check that appropriate types are defined. */ wchar_t a = 'c'; ptrdiff_t b = 1; size_t c = 2; max_align_t x; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); /* Check that offsetof produces integer constants with correct type. */ struct d { char e; char f; }; /* Solaris 10 has a bug where offsetof is under-parenthesized, and cannot be used as an arbitrary expression. However, since it is unlikely to bite real code, we ignore that short-coming. */ /* verify (sizeof offsetof (struct d, e) == sizeof (size_t)); */ verify (sizeof (offsetof (struct d, e)) == sizeof (size_t)); verify (offsetof (struct d, f) == 1); /* offsetof promotes to an unsigned integer if and only if sizes do not fit in int. */ verify ((offsetof (struct d, e) < -1) == (INT_MAX < (size_t) -1)); /* Check max_align_t's alignment. */ verify (alignof (double) <= alignof (max_align_t)); verify (alignof (int) <= alignof (max_align_t)); verify (alignof (long double) <= alignof (max_align_t)); verify (alignof (long int) <= alignof (max_align_t)); verify (alignof (ptrdiff_t) <= alignof (max_align_t)); verify (alignof (size_t) <= alignof (max_align_t)); verify (alignof (wchar_t) <= alignof (max_align_t)); verify (alignof (struct d) <= alignof (max_align_t)); #if defined __GNUC__ || defined __IBM__ALIGNOF__ verify (__alignof__ (double) <= __alignof__ (max_align_t)); verify (__alignof__ (int) <= __alignof__ (max_align_t)); verify (__alignof__ (long double) <= __alignof__ (max_align_t)); verify (__alignof__ (long int) <= __alignof__ (max_align_t)); verify (__alignof__ (ptrdiff_t) <= __alignof__ (max_align_t)); verify (__alignof__ (size_t) <= __alignof__ (max_align_t)); verify (__alignof__ (wchar_t) <= __alignof__ (max_align_t)); verify (__alignof__ (struct d) <= __alignof__ (max_align_t)); #endif int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-stdbool.c0000644000175000017500000000663613217200024016602 00000000000000/* Test of substitute. Copyright (C) 2002-2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ /* We want this test to succeed even when using gcc's -Werror; but to do that requires a pragma that didn't exist before 4.3.0. */ #ifndef __GNUC__ # define ADDRESS_CHECK_OKAY #elif __GNUC__ < 4 || (__GNUC__ == 4 && __GNUC_MINOR__ < 3) /* No way to silence -Waddress. */ #else # pragma GCC diagnostic ignored "-Waddress" # define ADDRESS_CHECK_OKAY #endif #include #include #ifndef bool "error: bool is not defined" #endif #ifndef false "error: false is not defined" #endif #if false "error: false is not 0" #endif #ifndef true "error: true is not defined" #endif #if true != 1 "error: true is not 1" #endif #ifndef __bool_true_false_are_defined "error: __bool_true_false_are_defined is not defined" #endif /* Several tests cannot be guaranteed with gnulib's , at least, not for all compilers and compiler options. */ #if HAVE_STDBOOL_H || 3 <= __GNUC__ struct s { _Bool s: 1; _Bool t; } s; #endif char a[true == 1 ? 1 : -1]; char b[false == 0 ? 1 : -1]; char c[__bool_true_false_are_defined == 1 ? 1 : -1]; #if HAVE_STDBOOL_H || 3 <= __GNUC__ /* See above. */ char d[(bool) 0.5 == true ? 1 : -1]; # ifdef ADDRESS_CHECK_OKAY /* Avoid gcc warning. */ /* C99 may plausibly be interpreted as not requiring support for a cast from a variable's address to bool in a static initializer. So treat it like a GCC extension. */ # ifdef __GNUC__ bool e = &s; # endif # endif char f[(_Bool) 0.0 == false ? 1 : -1]; #endif char g[true]; char h[sizeof (_Bool)]; #if HAVE_STDBOOL_H || 3 <= __GNUC__ /* See above. */ char i[sizeof s.t]; #endif enum { j = false, k = true, l = false * true, m = true * 256 }; _Bool n[m]; char o[sizeof n == m * sizeof n[0] ? 1 : -1]; char p[-1 - (_Bool) 0 < 0 && -1 - (bool) 0 < 0 ? 1 : -1]; /* Catch a bug in an HP-UX C compiler. See https://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html https://lists.gnu.org/r/bug-coreutils/2005-11/msg00161.html */ _Bool q = true; _Bool *pq = &q; int main () { int error = 0; #if HAVE_STDBOOL_H || 3 <= __GNUC__ /* See above. */ # ifdef ADDRESS_CHECK_OKAY /* Avoid gcc warning. */ /* A cast from a variable's address to bool is valid in expressions. */ { bool e1 = &s; if (!e1) error = 1; } # endif #endif /* Catch a bug in IBM AIX xlc compiler version 6.0.0.0 reported by James Lemley on 2005-10-05; see https://lists.gnu.org/r/bug-coreutils/2005-10/msg00086.html This is a runtime test, since a corresponding compile-time test would rely on initializer extensions. */ { char digs[] = "0123456789"; if (&(digs + 5)[-2 + (bool) 1] != &digs[4]) error = 1; } return error; } gnuastro-0.5/bootstrapped/tests/test-stdalign.c0000644000175000017500000000733213217200024016733 00000000000000/* Test of . Copyright 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert, inspired by Bruno Haible's test-alignof.c. */ #include #include #include #include #include "verify.h" #include "macros.h" typedef long double longdouble; typedef struct { char a[1]; } struct1; typedef struct { char a[2]; } struct2; typedef struct { char a[3]; } struct3; typedef struct { char a[4]; } struct4; verify (__alignof_is_defined == 1); #ifndef alignof # error "alignof is not a macro" #endif #if __alignas_is_defined verify (__alignas_is_defined == 1); # ifndef alignas # error "alignas is not a macro" # endif /* mingw can go up only to 8. 8 is all that GNU Emacs needs, so let's limit the test to 8 for now. */ # define TEST_ALIGNMENT 8 #else # define _Alignas(alignment) # define alignas(alignment) # define TEST_ALIGNMENT 1 #endif #define CHECK_STATIC(type) \ typedef struct { char slot1; type slot2; } type##_helper; \ verify (alignof (type) == offsetof (type##_helper, slot2)); \ verify (_Alignof (type) == alignof (type)); \ const int type##_alignment = alignof (type); \ type alignas (TEST_ALIGNMENT) static_##type##_alignas; \ type _Alignas (TEST_ALIGNMENT) static_##type##_Alignas #define CHECK_ALIGNED(var) ASSERT ((uintptr_t) &(var) % TEST_ALIGNMENT == 0) CHECK_STATIC (char); CHECK_STATIC (short); CHECK_STATIC (int); CHECK_STATIC (long); #ifdef INT64_MAX CHECK_STATIC (int64_t); #endif CHECK_STATIC (float); CHECK_STATIC (double); /* CHECK_STATIC (longdouble); */ CHECK_STATIC (struct1); CHECK_STATIC (struct2); CHECK_STATIC (struct3); CHECK_STATIC (struct4); int main () { #if defined __SUNPRO_C /* Avoid a test failure due to Sun Studio Developer Bug Report #2125432. */ fputs ("Skipping test: known Sun C compiler bug\n", stderr); return 77; #elif defined __HP_cc && __ia64 /* Avoid a test failure due to HP-UX Itanium cc bug; see: https://lists.gnu.org/r/bug-gnulib/2017-03/msg00078.html */ fputs ("Skipping test: known HP-UX Itanium cc compiler bug\n", stderr); return 77; #else CHECK_ALIGNED (static_char_alignas); CHECK_ALIGNED (static_char_Alignas); CHECK_ALIGNED (static_short_alignas); CHECK_ALIGNED (static_short_Alignas); CHECK_ALIGNED (static_int_alignas); CHECK_ALIGNED (static_int_Alignas); CHECK_ALIGNED (static_long_alignas); CHECK_ALIGNED (static_long_Alignas); # ifdef INT64_MAX CHECK_ALIGNED (static_int64_t_alignas); CHECK_ALIGNED (static_int64_t_Alignas); # endif CHECK_ALIGNED (static_float_alignas); CHECK_ALIGNED (static_float_Alignas); CHECK_ALIGNED (static_double_alignas); CHECK_ALIGNED (static_double_Alignas); /* CHECK_ALIGNED (static_longdouble_alignas); */ /* CHECK_ALIGNED (static_longdouble_Alignas); */ CHECK_ALIGNED (static_struct1_alignas); CHECK_ALIGNED (static_struct1_Alignas); CHECK_ALIGNED (static_struct2_alignas); CHECK_ALIGNED (static_struct2_Alignas); CHECK_ALIGNED (static_struct3_alignas); CHECK_ALIGNED (static_struct3_Alignas); CHECK_ALIGNED (static_struct4_alignas); CHECK_ALIGNED (static_struct4_Alignas); return 0; #endif } gnuastro-0.5/bootstrapped/tests/test-stat-time.c0000644000175000017500000001527013217200024017035 00000000000000/* Test of . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by James Youngman , 2007. */ #include #include "stat-time.h" #include #include #include #include #include #include #include "macros.h" #define BASE "test-stat-time.t" #include "nap.h" enum { NFILES = 4 }; static char filename_stamp1[50]; static char filename_testfile[50]; static char filename_stamp2[50]; static char filename_stamp3[50]; /* Use file names that are different at each run. This is necessary for test_birthtime() to pass on native Windows: On this platform, the file system apparently remembers the creation time of a file even after it is removed and created anew. See "Windows NT Contains File System Tunneling Capabilities" */ static void initialize_filenames (void) { long t = (long) time (NULL); sprintf (filename_stamp1, "t-stt-%ld-stamp1", t); sprintf (filename_testfile, "t-stt-%ld-testfile", t); sprintf (filename_stamp2, "t-stt-%ld-stamp2", t); sprintf (filename_stamp3, "t-stt-%ld-stamp3", t); } static int force_unlink (const char *filename) { /* This chmod is necessary on mingw, where unlink() of a read-only file fails with EPERM. */ chmod (filename, 0600); return unlink (filename); } static void cleanup (int sig) { /* Remove temporary files. */ force_unlink (filename_stamp1); force_unlink (filename_testfile); force_unlink (filename_stamp2); force_unlink (filename_stamp3); if (sig != 0) _exit (1); } static int open_file (const char *filename, int flags) { int fd = open (filename, flags | O_WRONLY, 0500); if (fd >= 0) { close (fd); return 1; } else { return 0; } } static void create_file (const char *filename) { ASSERT (open_file (filename, O_CREAT | O_EXCL)); } static void do_stat (const char *filename, struct stat *p) { ASSERT (stat (filename, p) == 0); } static void prepare_test (struct stat *statinfo, struct timespec *modtimes) { int i; create_file (filename_stamp1); nap (); create_file (filename_testfile); nap (); create_file (filename_stamp2); nap (); ASSERT (chmod (filename_testfile, 0400) == 0); nap (); create_file (filename_stamp3); do_stat (filename_stamp1, &statinfo[0]); do_stat (filename_testfile, &statinfo[1]); do_stat (filename_stamp2, &statinfo[2]); do_stat (filename_stamp3, &statinfo[3]); /* Now use our access functions. */ for (i = 0; i < NFILES; ++i) { modtimes[i] = get_stat_mtime (&statinfo[i]); } } static void test_mtime (const struct stat *statinfo, struct timespec *modtimes) { int i; /* Use the struct stat fields directly. */ /* mtime(stamp1) < mtime(stamp2) */ ASSERT (statinfo[0].st_mtime < statinfo[2].st_mtime || (statinfo[0].st_mtime == statinfo[2].st_mtime && (get_stat_mtime_ns (&statinfo[0]) < get_stat_mtime_ns (&statinfo[2])))); /* mtime(stamp2) < mtime(stamp3) */ ASSERT (statinfo[2].st_mtime < statinfo[3].st_mtime || (statinfo[2].st_mtime == statinfo[3].st_mtime && (get_stat_mtime_ns (&statinfo[2]) < get_stat_mtime_ns (&statinfo[3])))); /* Now check the result of the access functions. */ /* mtime(stamp1) < mtime(stamp2) */ ASSERT (modtimes[0].tv_sec < modtimes[2].tv_sec || (modtimes[0].tv_sec == modtimes[2].tv_sec && modtimes[0].tv_nsec < modtimes[2].tv_nsec)); /* mtime(stamp2) < mtime(stamp3) */ ASSERT (modtimes[2].tv_sec < modtimes[3].tv_sec || (modtimes[2].tv_sec == modtimes[3].tv_sec && modtimes[2].tv_nsec < modtimes[3].tv_nsec)); /* verify equivalence */ for (i = 0; i < NFILES; ++i) { struct timespec ts; ts = get_stat_mtime (&statinfo[i]); ASSERT (ts.tv_sec == statinfo[i].st_mtime); } } #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* Skip the ctime tests on native Windows platforms, because their st_ctime is either the same as st_mtime (plus or minus an offset) or set to the file _creation_ time, and is not influenced by rename or chmod. */ # define test_ctime(ignored) ((void) 0) #else static void test_ctime (const struct stat *statinfo) { /* On some buggy NFS clients, mtime and ctime are disproportionately skewed from one another. Skip this test in that case. */ if (statinfo[0].st_mtime != statinfo[0].st_ctime) return; /* mtime(stamp2) < ctime(testfile) */ ASSERT (statinfo[2].st_mtime < statinfo[1].st_ctime || (statinfo[2].st_mtime == statinfo[1].st_ctime && (get_stat_mtime_ns (&statinfo[2]) < get_stat_ctime_ns (&statinfo[1])))); } #endif static void test_birthtime (const struct stat *statinfo, const struct timespec *modtimes, struct timespec *birthtimes) { int i; /* Collect the birth times. */ for (i = 0; i < NFILES; ++i) { birthtimes[i] = get_stat_birthtime (&statinfo[i]); if (birthtimes[i].tv_nsec < 0) return; } /* mtime(stamp1) < birthtime(testfile) */ ASSERT (modtimes[0].tv_sec < birthtimes[1].tv_sec || (modtimes[0].tv_sec == birthtimes[1].tv_sec && modtimes[0].tv_nsec < birthtimes[1].tv_nsec)); /* birthtime(testfile) < mtime(stamp2) */ ASSERT (birthtimes[1].tv_sec < modtimes[2].tv_sec || (birthtimes[1].tv_sec == modtimes[2].tv_sec && birthtimes[1].tv_nsec < modtimes[2].tv_nsec)); } int main (void) { struct stat statinfo[NFILES]; struct timespec modtimes[NFILES]; struct timespec birthtimes[NFILES]; initialize_filenames (); #ifdef SIGHUP signal (SIGHUP, cleanup); #endif #ifdef SIGINT signal (SIGINT, cleanup); #endif #ifdef SIGQUIT signal (SIGQUIT, cleanup); #endif #ifdef SIGTERM signal (SIGTERM, cleanup); #endif cleanup (0); prepare_test (statinfo, modtimes); test_mtime (statinfo, modtimes); test_ctime (statinfo); test_birthtime (statinfo, modtimes, birthtimes); cleanup (0); return 0; } gnuastro-0.5/bootstrapped/tests/test-stat.c0000644000175000017500000000313413217200024016075 00000000000000/* Tests of stat. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include /* Caution: stat may be a function-like macro. Although this signature check must pass, it may be the signature of the real (and broken) stat rather than rpl_stat. Most code should not use the address of stat. */ #include "signature.h" SIGNATURE_CHECK (stat, int, (char const *, struct stat *)); #include #include #include #include #include #include #include "same-inode.h" #include "macros.h" #define BASE "test-stat.t" #include "test-stat.h" /* Wrapper around stat, which works even if stat is a function-like macro, where test_stat_func(stat) would do the wrong thing. */ static int do_stat (char const *name, struct stat *st) { return stat (name, st); } int main (void) { return test_stat_func (do_stat, true); } gnuastro-0.5/bootstrapped/tests/test-sockets.c0000644000175000017500000000216413217200024016577 00000000000000/* * Copyright (C) 2008-2017 Free Software Foundation, Inc. * Written by Simon Josefsson. * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "sockets.h" int main (void) { int err; err = gl_sockets_startup (SOCKETS_1_1); if (err != 0) { printf ("wsastartup failed %d\n", err); return 1; } err = gl_sockets_cleanup (); if (err != 0) { printf ("wsacleanup failed %d\n", err); return 1; } (void) gl_fd_to_handle (0); return 0; } gnuastro-0.5/bootstrapped/tests/test-sleep.c0000644000175000017500000000263313217200024016235 00000000000000/* Test of sleep() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (sleep, unsigned int, (unsigned int)); #include #include "macros.h" #if HAVE_DECL_ALARM static void handle_alarm (int sig) { if (sig != SIGALRM) _exit (1); } #endif int main (void) { ASSERT (sleep (1) <= 1); ASSERT (sleep (0) == 0); #if HAVE_DECL_ALARM { const unsigned int pentecost = 50 * 24 * 60 * 60; /* 50 days. */ unsigned int remaining; signal (SIGALRM, handle_alarm); alarm (1); remaining = sleep (pentecost); ASSERT (pentecost - 10 < remaining && remaining <= pentecost); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-sigprocmask.c0000644000175000017500000000510713217200024017446 00000000000000/* Test of sigprocmask. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include #include "signature.h" SIGNATURE_CHECK (sigprocmask, int, (int, const sigset_t *, sigset_t *)); #include #include #include #include #include "macros.h" #if !((defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__) static volatile int sigint_occurred; static void sigint_handler (int sig) { sigint_occurred++; } int main (int argc, char *argv[]) { sigset_t set; pid_t pid = getpid (); char command[80]; if (sizeof (int) < sizeof pid && 0x7fffffff < pid) { fputs ("Skipping test: pid too large\n", stderr); return 77; } signal (SIGINT, sigint_handler); sigemptyset (&set); sigaddset (&set, SIGINT); /* Check error handling. */ ASSERT (sigprocmask (1729, &set, NULL) == -1); ASSERT (errno == EINVAL); /* Block SIGINT. */ ASSERT (sigprocmask (SIG_BLOCK, &set, NULL) == 0); /* Request a SIGINT signal from outside. */ sprintf (command, "sh -c 'sleep 1; kill -%d %d' &", SIGINT, (int) pid); ASSERT (system (command) == 0); /* Wait. */ sleep (2); /* The signal should not have arrived yet, because it is blocked. */ ASSERT (sigint_occurred == 0); /* Unblock SIGINT. */ ASSERT (sigprocmask (SIG_UNBLOCK, &set, NULL) == 0); /* The signal should have arrived now, because POSIX says "If there are any pending unblocked signals after the call to sigprocmask(), at least one of those signals shall be delivered before the call to sigprocmask() returns." */ ASSERT (sigint_occurred == 1); return 0; } #else /* On native Windows, getpid() values and the arguments that are passed to the (Cygwin?) 'kill' program are not necessarily related. */ int main () { fputs ("Skipping test: native Windows platform\n", stderr); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-signbit.c0000644000175000017500000001267313217200024016571 00000000000000/* Test of signbit() substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include /* signbit must be a macro. */ #ifndef signbit # error missing declaration #endif #include #include #include "minus-zero.h" #include "infinity.h" #include "macros.h" float zerof = 0.0f; double zerod = 0.0; long double zerol = 0.0L; static void test_signbitf () { /* Finite values. */ ASSERT (!signbit (3.141f)); ASSERT (!signbit (3.141e30f)); ASSERT (!signbit (3.141e-30f)); ASSERT (signbit (-2.718f)); ASSERT (signbit (-2.718e30f)); ASSERT (signbit (-2.718e-30f)); /* Zeros. */ ASSERT (!signbit (0.0f)); if (1.0f / minus_zerof < 0) ASSERT (signbit (minus_zerof)); else ASSERT (!signbit (minus_zerof)); /* Infinite values. */ ASSERT (!signbit (Infinityf ())); ASSERT (signbit (- Infinityf ())); /* Quiet NaN. */ (void) signbit (zerof / zerof); #if defined FLT_EXPBIT0_WORD && defined FLT_EXPBIT0_BIT /* Signalling NaN. */ { #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; memory_float m; m.value = zerof / zerof; # if FLT_EXPBIT0_BIT > 0 m.word[FLT_EXPBIT0_WORD] ^= (unsigned int) 1 << (FLT_EXPBIT0_BIT - 1); # else m.word[FLT_EXPBIT0_WORD + (FLT_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); # endif if (FLT_EXPBIT0_WORD < NWORDS / 2) m.word[FLT_EXPBIT0_WORD + 1] |= (unsigned int) 1 << FLT_EXPBIT0_BIT; else m.word[0] |= (unsigned int) 1; (void) signbit (m.value); #undef NWORDS } #endif } static void test_signbitd () { /* Finite values. */ ASSERT (!signbit (3.141)); ASSERT (!signbit (3.141e30)); ASSERT (!signbit (3.141e-30)); ASSERT (signbit (-2.718)); ASSERT (signbit (-2.718e30)); ASSERT (signbit (-2.718e-30)); /* Zeros. */ ASSERT (!signbit (0.0)); if (1.0 / minus_zerod < 0) ASSERT (signbit (minus_zerod)); else ASSERT (!signbit (minus_zerod)); /* Infinite values. */ ASSERT (!signbit (Infinityd ())); ASSERT (signbit (- Infinityd ())); /* Quiet NaN. */ (void) signbit (zerod / zerod); #if defined DBL_EXPBIT0_WORD && defined DBL_EXPBIT0_BIT /* Signalling NaN. */ { #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; memory_double m; m.value = zerod / zerod; # if DBL_EXPBIT0_BIT > 0 m.word[DBL_EXPBIT0_WORD] ^= (unsigned int) 1 << (DBL_EXPBIT0_BIT - 1); # else m.word[DBL_EXPBIT0_WORD + (DBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); # endif m.word[DBL_EXPBIT0_WORD + (DBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] |= (unsigned int) 1 << DBL_EXPBIT0_BIT; (void) signbit (m.value); #undef NWORDS } #endif } static void test_signbitl () { /* Finite values. */ ASSERT (!signbit (3.141L)); ASSERT (!signbit (3.141e30L)); ASSERT (!signbit (3.141e-30L)); ASSERT (signbit (-2.718L)); ASSERT (signbit (-2.718e30L)); ASSERT (signbit (-2.718e-30L)); /* Zeros. */ ASSERT (!signbit (0.0L)); if (1.0L / minus_zerol < 0) ASSERT (signbit (minus_zerol)); else ASSERT (!signbit (minus_zerol)); /* Infinite values. */ ASSERT (!signbit (Infinityl ())); ASSERT (signbit (- Infinityl ())); /* Quiet NaN. */ (void) signbit (zerol / zerol); #if defined LDBL_EXPBIT0_WORD && defined LDBL_EXPBIT0_BIT /* Signalling NaN. */ { #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { long double value; unsigned int word[NWORDS]; } memory_long_double; #if defined __powerpc__ && LDBL_MANT_DIG == 106 /* This is PowerPC "double double", a pair of two doubles. Inf and Nan are represented as the corresponding 64-bit IEEE values in the first double; the second is ignored. Manipulate only the first double. */ #undef NWORDS #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) #endif memory_long_double m; m.value = zerol / zerol; # if LDBL_EXPBIT0_BIT > 0 m.word[LDBL_EXPBIT0_WORD] ^= (unsigned int) 1 << (LDBL_EXPBIT0_BIT - 1); # else m.word[LDBL_EXPBIT0_WORD + (LDBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); # endif m.word[LDBL_EXPBIT0_WORD + (LDBL_EXPBIT0_WORD < NWORDS / 2 ? 1 : - 1)] |= (unsigned int) 1 << LDBL_EXPBIT0_BIT; (void) signbit (m.value); #undef NWORDS } #endif } int main () { test_signbitf (); test_signbitd (); test_signbitl (); return 0; } gnuastro-0.5/bootstrapped/tests/test-signal-h.c0000644000175000017500000000475313217200024016634 00000000000000/* Test of substitute. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include /* Check for required types. */ struct { size_t a; uid_t b; volatile sig_atomic_t c; sigset_t d; pid_t e; #if 0 /* Not guaranteed by gnulib. */ pthread_t f; struct timespec g; #endif } s; /* Check that NSIG is defined. */ int nsig = NSIG; int main (void) { switch (0) { /* The following are guaranteed by C. */ case 0: case SIGABRT: case SIGFPE: case SIGILL: case SIGINT: case SIGSEGV: case SIGTERM: /* The following is guaranteed by gnulib. */ #if GNULIB_SIGPIPE || defined SIGPIPE case SIGPIPE: #endif /* Ensure no conflict with other standardized names. */ #ifdef SIGALRM case SIGALRM: #endif /* On Haiku, SIGBUS is mistakenly equal to SIGSEGV. */ #if defined SIGBUS && SIGBUS != SIGSEGV case SIGBUS: #endif #ifdef SIGCHLD case SIGCHLD: #endif #ifdef SIGCONT case SIGCONT: #endif #ifdef SIGHUP case SIGHUP: #endif #ifdef SIGKILL case SIGKILL: #endif #ifdef SIGQUIT case SIGQUIT: #endif #ifdef SIGSTOP case SIGSTOP: #endif #ifdef SIGTSTP case SIGTSTP: #endif #ifdef SIGTTIN case SIGTTIN: #endif #ifdef SIGTTOU case SIGTTOU: #endif #ifdef SIGUSR1 case SIGUSR1: #endif #ifdef SIGUSR2 case SIGUSR2: #endif #ifdef SIGSYS case SIGSYS: #endif #ifdef SIGTRAP case SIGTRAP: #endif #ifdef SIGURG case SIGURG: #endif #ifdef SIGVTALRM case SIGVTALRM: #endif #ifdef SIGXCPU case SIGXCPU: #endif #ifdef SIGXFSZ case SIGXFSZ: #endif /* SIGRTMIN and SIGRTMAX need not be compile-time constants. */ #if 0 # ifdef SIGRTMIN case SIGRTMIN: # endif # ifdef SIGRTMAX case SIGRTMAX: # endif #endif ; } return s.a + s.b + s.c + s.e; } gnuastro-0.5/bootstrapped/tests/test-sigaction.c0000644000175000017500000000677513217200024017120 00000000000000/* Test of sigaction() function. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (sigaction, int, (int, struct sigaction const *, struct sigaction *)); #include #include "macros.h" #ifndef SA_NOCLDSTOP # define SA_NOCLDSTOP 0 #endif #ifndef SA_ONSTACK # define SA_ONSTACK 0 #endif #ifndef SA_RESETHAND # define SA_RESETHAND 0 #endif #ifndef SA_RESTART # define SA_RESTART 0 #endif #ifndef SA_SIGINFO # define SA_SIGINFO 0 #endif #ifndef SA_NOCLDWAIT # define SA_NOCLDWAIT 0 #endif /* Define a mask of flags required by POSIX. Some implementations provide other flags as extensions, such as SA_RESTORER, that we must ignore in this test. */ #define MASK_SA_FLAGS (SA_NOCLDSTOP | SA_ONSTACK | SA_RESETHAND | SA_RESTART \ | SA_SIGINFO | SA_NOCLDWAIT | SA_NODEFER) /* This test is unsafe in the presence of an asynchronous SIGABRT, because we install a signal-handler that is intentionally not async-safe. Hopefully, this does not lead to too many reports of false failures, since people don't generally use 'kill -s SIGABRT' to end a runaway program. */ static void handler (int sig) { static int entry_count; struct sigaction sa; ASSERT (sig == SIGABRT); ASSERT (sigaction (SIGABRT, NULL, &sa) == 0); ASSERT ((sa.sa_flags & SA_SIGINFO) == 0); switch (entry_count++) { case 0: ASSERT ((sa.sa_flags & SA_RESETHAND) == 0); ASSERT (sa.sa_handler == handler); break; case 1: /* This assertion fails on glibc-2.3.6 systems with LinuxThreads, when this program is linked with -lpthread, due to the sigaction() override in libpthread.so. */ #if !(defined __GLIBC__ || defined __UCLIBC__) ASSERT (sa.sa_handler == SIG_DFL); #endif break; default: ASSERT (0); } } int main (void) { struct sigaction sa; struct sigaction old_sa; sa.sa_handler = handler; sa.sa_flags = 0; ASSERT (sigemptyset (&sa.sa_mask) == 0); ASSERT (sigaction (SIGABRT, &sa, NULL) == 0); ASSERT (raise (SIGABRT) == 0); sa.sa_flags = SA_RESETHAND | SA_NODEFER; ASSERT (sigaction (SIGABRT, &sa, &old_sa) == 0); ASSERT ((old_sa.sa_flags & MASK_SA_FLAGS) == 0); ASSERT (old_sa.sa_handler == handler); ASSERT (raise (SIGABRT) == 0); sa.sa_handler = SIG_DFL; ASSERT (sigaction (SIGABRT, &sa, &old_sa) == 0); ASSERT ((old_sa.sa_flags & SA_SIGINFO) == 0); #if !(defined __GLIBC__ || defined __UCLIBC__) /* see above */ ASSERT (old_sa.sa_handler == SIG_DFL); #endif sa.sa_handler = SIG_IGN; ASSERT (sigaction (SIGABRT, &sa, NULL) == 0); ASSERT (raise (SIGABRT) == 0); ASSERT (sigaction (SIGABRT, NULL, &old_sa) == 0); ASSERT (old_sa.sa_handler == SIG_IGN); ASSERT (raise (SIGABRT) == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-setsockopt.c0000644000175000017500000000265613217200024017330 00000000000000/* Test setsockopt() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (setsockopt, int, (int, int, int, const void *, socklen_t)); #include #include #include "sockets.h" #include "macros.h" int main (void) { (void) gl_sockets_startup (SOCKETS_1_1); /* Test behaviour for invalid file descriptors. */ { int value = 1; errno = 0; ASSERT (setsockopt (-1, SOL_SOCKET, SO_REUSEADDR, &value, sizeof (value)) == -1); ASSERT (errno == EBADF); } { int value = 1; close (99); errno = 0; ASSERT (setsockopt (99, SOL_SOCKET, SO_REUSEADDR, &value, sizeof (value)) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.5/bootstrapped/tests/test-setlocale2.c0000644000175000017500000000335013217200024017157 00000000000000/* Test of setting the current locale. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include int main () { /* Try to set the locale by implicitly looking at the LC_ALL environment variable. */ if (setlocale (LC_ALL, "") != NULL) /* It was successful. Check whether LC_CTYPE is non-trivial. */ if (strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) { fprintf (stderr, "setlocale did not fail for implicit %s\n", getenv ("LC_ALL")); return 1; } /* Reset the locale. */ if (setlocale (LC_ALL, "C") == NULL) return 1; /* Try to set the locale by explicitly looking at the LC_ALL environment variable. */ if (setlocale (LC_ALL, getenv ("LC_ALL")) != NULL) /* It was successful. Check whether LC_CTYPE is non-trivial. */ if (strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) { fprintf (stderr, "setlocale did not fail for explicit %s\n", getenv ("LC_ALL")); return 1; } return 0; } gnuastro-0.5/bootstrapped/tests/test-setlocale1.c0000644000175000017500000000334213217200024017157 00000000000000/* Test of setting the current locale. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (setlocale, char *, (int, const char *)); #include #include #include "macros.h" int main (int argc, char *argv[]) { char *name1; char *name2; /* Try to set the locale by implicitly looking at the LC_ALL environment variable. configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; name1 = strdup (setlocale (LC_ALL, NULL)); /* Reset the locale. */ if (setlocale (LC_ALL, "C") == NULL) return 1; /* Try to set the locale by explicitly looking at the LC_ALL environment variable. configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL) return 1; name2 = strdup (setlocale (LC_ALL, NULL)); /* Test that the two results are the same. */ ASSERT (strcmp (name1, name2) == 0); free (name1); free (name2); return 0; } gnuastro-0.5/bootstrapped/tests/test-setenv.c0000644000175000017500000000310713217200024016426 00000000000000/* Tests of setenv. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (setenv, int, (char const *, char const *, int)); #include #include #include #include "macros.h" int main (void) { /* Test overwriting. */ ASSERT (setenv ("a", "==", -1) == 0); ASSERT (setenv ("a", "2", 0) == 0); ASSERT (strcmp (getenv ("a"), "==") == 0); /* Required to fail with EINVAL. */ errno = 0; ASSERT (setenv ("", "", 1) == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (setenv ("a=b", "", 0) == -1); ASSERT (errno == EINVAL); #if 0 /* glibc and gnulib's implementation guarantee this, but POSIX no longer requires it: http://austingroupbugs.net/view.php?id=185 */ errno = 0; ASSERT (setenv (NULL, "", 0) == -1); ASSERT (errno == EINVAL); #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-select-stdin.c0000644000175000017500000000433313217200024017522 00000000000000/* Test of select() substitute, reading from stdin. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include #include #include #include #include "macros.h" int main (void) { printf ("Applying select() from standard input. Press Ctrl-C to abort.\n"); for (;;) { struct timeval before; struct timeval after; unsigned long spent_usec; fd_set readfds; struct timeval timeout; int ret; gettimeofday (&before, NULL); FD_ZERO (&readfds); FD_SET (0, &readfds); timeout.tv_sec = 0; timeout.tv_usec = 500000; ret = select (1, &readfds, NULL, NULL, &timeout); gettimeofday (&after, NULL); spent_usec = (after.tv_sec - before.tv_sec) * 1000000 + after.tv_usec - before.tv_usec; if (ret < 0) { perror ("select failed"); exit (1); } if ((ret == 0) != ! FD_ISSET (0, &readfds)) { fprintf (stderr, "incorrect return value\n"); exit (1); } if (ret == 0) { if (spent_usec < 250000) { fprintf (stderr, "returned too early\n"); exit (1); } /* Timeout */ printf ("."); ASSERT (fflush (stdout) == 0); } else { char c; printf ("Input available! Trying to read 1 byte...\n"); ASSERT (read (0, &c, 1) == 1); } } } gnuastro-0.5/bootstrapped/tests/test-select-fd.c0000644000175000017500000000442613217200024016775 00000000000000/* Test of select() substitute, reading or writing from a given file descriptor. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include #include int main (int argc, char *argv[]) { if (argc == 4) { char mode = argv[1][0]; if (mode == 'r' || mode == 'w') { int fd = atoi (argv[2]); if (fd >= 0) { const char *result_file_name = argv[3]; FILE *result_file = fopen (result_file_name, "wb"); if (result_file != NULL) { fd_set fds; struct timeval timeout; int ret; FD_ZERO (&fds); FD_SET (fd, &fds); timeout.tv_sec = 0; timeout.tv_usec = 10000; ret = (mode == 'r' ? select (fd + 1, &fds, NULL, NULL, &timeout) : select (fd + 1, NULL, &fds, NULL, &timeout)); if (ret < 0) { perror ("select failed"); exit (1); } if ((ret == 0) != ! FD_ISSET (fd, &fds)) { fprintf (stderr, "incorrect return value\n"); exit (1); } fprintf (result_file, "%d\n", ret); exit (0); } } } } fprintf (stderr, "Usage: test-select-fd mode fd result-file-name\n"); exit (1); } gnuastro-0.5/bootstrapped/tests/test-select.c0000644000175000017500000000202613217200024016400 00000000000000/* Test of select() substitute. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini, 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (select, int, (int, fd_set *, fd_set *, fd_set *, struct timeval *)); #include "test-select.h" int main (void) { return test_function (select); } gnuastro-0.5/bootstrapped/tests/test-rwlock1.c0000644000175000017500000001243313217200024016506 00000000000000/* Test of glthread_rwlock_rdlock function. Copyright (C) 2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. Inspired by https://github.com/linux-test-project/ltp/blob/master/testcases/open_posix_testsuite/conformance/interfaces/pthread_rwlock_rdlock/2-2.c by Intel Corporation. */ #include #include "glthread/lock.h" #include #include #include #include #include "glthread/thread.h" #include "glthread/yield.h" /* Verify that in a situation where - an rwlock is taken by a reader and has a writer waiting, - an additional reader requests the lock, - the waiting writer and the requesting reader threads have the same priority, the requesting reader thread gets blocked, so that at some point the waiting writer can acquire the lock. Without such a guarantee, when there a N readers and each of the readers spends more than 1/Nth of the time with the lock held, there is a high probability that the waiting writer will not get the lock in a given finite time, a phenomenon called "writer starvation". Without such a guarantee, applications have a hard time avoiding writer starvation. POSIX:2008 makes this requirement only for implementations that support TPS (Thread Priority Scheduling) and only for the scheduling policies SCHED_FIFO and SCHED_RR, see http://pubs.opengroup.org/onlinepubs/9699919799/functions/pthread_rwlock_rdlock.html but test verifies the guarantee regardless of TPS and regardless of scheduling policy. */ #define SUCCEED() exit (0) #define FAILURE() exit (1) #define UNEXPECTED(n) (fprintf (stderr, "Unexpected outcome %d\n", n), abort ()) /* The main thread creates the waiting writer and the requesting reader threads in the default way; this guarantees that they have the same priority. We can reuse the main thread as first reader thread. */ static gl_rwlock_t lock; static gl_thread_t reader1; static gl_thread_t writer; static gl_thread_t reader2; static gl_thread_t timer; /* Used to pass control from writer to reader2 and from reader2 to timer, as in a relay race. Passing control from one running thread to another running thread is most likely faster than to create the second thread. */ static gl_lock_t baton; static void * timer_func (void *ignored) { /* Step 13 (can be before or after step 12): The timer thread takes the baton, then waits a moment to make sure it can tell whether the second reader thread is blocked at step 12. */ if (glthread_lock_lock (&baton)) UNEXPECTED (13); usleep (100000); /* By the time we get here, it's clear that the second reader thread is blocked at step 12. This is the desired behaviour. */ SUCCEED (); } static void * reader2_func (void *ignored) { int err; /* Step 8 (can be before or after step 7): The second reader thread takes the baton, then waits a moment to make sure the writer thread has reached step 7. */ if (glthread_lock_lock (&baton)) UNEXPECTED (8); usleep (100000); /* Step 9 omitted. */ /* Step 10: Launch a timer, to test whether the next call blocks. */ if (glthread_create (&timer, timer_func, NULL)) UNEXPECTED (10); /* Step 11: Release the baton. */ if (glthread_lock_unlock (&baton)) UNEXPECTED (11); /* Step 12: The second reader thread requests the lock. */ err = glthread_rwlock_rdlock (&lock); if (err == 0) FAILURE (); else UNEXPECTED (12); } static void * writer_func (void *ignored) { /* Step 4: Take the baton, so that the second reader thread does not go ahead too early. */ if (glthread_lock_lock (&baton)) UNEXPECTED (4); /* Step 5: Create the second reader thread. */ if (glthread_create (&reader2, reader2_func, NULL)) UNEXPECTED (5); /* Step 6: Release the baton. */ if (glthread_lock_unlock (&baton)) UNEXPECTED (6); /* Step 7: The writer thread requests the lock. */ if (glthread_rwlock_wrlock (&lock)) UNEXPECTED (7); return NULL; } int main () { reader1 = gl_thread_self (); /* Step 1: The main thread initializes the lock and the baton. */ if (glthread_rwlock_init (&lock)) UNEXPECTED (1); if (glthread_lock_init (&baton)) UNEXPECTED (1); /* Step 2: The main thread acquires the lock as a reader. */ if (glthread_rwlock_rdlock (&lock)) UNEXPECTED (2); /* Step 3: Create the writer thread. */ if (glthread_create (&writer, writer_func, NULL)) UNEXPECTED (3); /* Job done. Go to sleep. */ for (;;) { /* In cooperative threads implementations (Pth), give other threads a chance to run. */ gl_thread_yield (); sleep (1); } } gnuastro-0.5/bootstrapped/tests/test-regex.c0000644000175000017500000001700513217200024016236 00000000000000/* Test regular expressions Copyright 1996-2001, 2003-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "regex.h" #include #include #include #include #if HAVE_DECL_ALARM # include # include #endif #include "localcharset.h" int main (void) { int result = 0; static struct re_pattern_buffer regex; unsigned char folded_chars[UCHAR_MAX + 1]; int i; const char *s; struct re_registers regs; #if HAVE_DECL_ALARM /* Some builds of glibc go into an infinite loop on this test. */ int alarm_value = 2; signal (SIGALRM, SIG_DFL); alarm (alarm_value); #endif if (setlocale (LC_ALL, "en_US.UTF-8")) { { /* https://sourceware.org/ml/libc-hacker/2006-09/msg00008.html This test needs valgrind to catch the bug on Debian GNU/Linux 3.1 x86, but it might catch the bug better on other platforms and it shouldn't hurt to try the test here. */ static char const pat[] = "insert into"; static char const data[] = "\xFF\0\x12\xA2\xAA\xC4\xB1,K\x12\xC4\xB1*\xACK"; re_set_syntax (RE_SYNTAX_GREP | RE_HAT_LISTS_NOT_NEWLINE | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { memset (®s, 0, sizeof regs); if (re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, ®s) != -1) result |= 1; regfree (®ex); free (regs.start); free (regs.end); } } /* Check whether it's really a UTF-8 locale. On mingw, the setlocale call succeeds but returns "English_United States.1252", with locale_charset() returning "CP1252". */ if (strcmp (locale_charset (), "UTF-8") == 0) { /* This test is from glibc bug 15078. The test case is from Andreas Schwab in . */ static char const pat[] = "[^x]x"; static char const data[] = /* */ "\xe1\x80\x80" "\xe1\x80\xbb" "\xe1\x80\xbd" "\xe1\x80\x94" "\xe1\x80\xba" "\xe1\x80\xaf" "\xe1\x80\x95" "\xe1\x80\xba" "x"; re_set_syntax (0); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { memset (®s, 0, sizeof regs); i = re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, 0); if (i != 0 && i != 21) result |= 1; regfree (®ex); free (regs.start); free (regs.end); } } if (! setlocale (LC_ALL, "C")) return 1; } /* This test is from glibc bug 3957, reported by Andrew Mackey. */ re_set_syntax (RE_SYNTAX_EGREP | RE_HAT_LISTS_NOT_NEWLINE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[^x]b", 6, ®ex); if (s) result |= 2; /* This should fail, but succeeds for glibc-2.5. */ else { memset (®s, 0, sizeof regs); if (re_search (®ex, "a\nb", 3, 0, 3, ®s) != -1) result |= 2; regfree (®ex); free (regs.start); free (regs.end); } /* This regular expression is from Spencer ere test number 75 in grep-2.3. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP); memset (®ex, 0, sizeof regex); for (i = 0; i <= UCHAR_MAX; i++) folded_chars[i] = i; regex.translate = folded_chars; s = re_compile_pattern ("a[[:@:>@:]]b\n", 11, ®ex); /* This should fail with _Invalid character class name_ error. */ if (!s) { result |= 4; regfree (®ex); } /* Ensure that [b-a] is diagnosed as invalid, when using RE_NO_EMPTY_RANGES. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP | RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[b-a]", 6, ®ex); if (s == 0) { result |= 8; regfree (®ex); } /* This should succeed, but does not for glibc-2.1.3. */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("{1", 2, ®ex); if (s) result |= 8; else regfree (®ex); /* The following example is derived from a problem report against gawk from Jorge Stolfi . */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[an\371]*n", 7, ®ex); if (s) result |= 8; /* This should match, but does not for glibc-2.2.1. */ else { memset (®s, 0, sizeof regs); if (re_match (®ex, "an", 2, 0, ®s) != 2) result |= 8; regfree (®ex); free (regs.start); free (regs.end); } memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 8; /* glibc-2.2.93 does not work with a negative RANGE argument. */ else { memset (®s, 0, sizeof regs); if (re_search (®ex, "wxy", 3, 2, -2, ®s) != 1) result |= 8; regfree (®ex); free (regs.start); free (regs.end); } /* The version of regex.c in older versions of gnulib ignored RE_ICASE. Detect that problem too. */ re_set_syntax (RE_SYNTAX_EMACS | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 16; else { memset (®s, 0, sizeof regs); if (re_search (®ex, "WXY", 3, 0, 3, ®s) < 0) result |= 16; regfree (®ex); free (regs.start); free (regs.end); } /* Catch a bug reported by Vin Shelton in https://lists.gnu.org/r/bug-coreutils/2007-06/msg00089.html */ re_set_syntax (RE_SYNTAX_POSIX_BASIC & ~RE_CONTEXT_INVALID_DUP & ~RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[[:alnum:]_-]\\\\+$", 16, ®ex); if (s) result |= 32; else regfree (®ex); /* REG_STARTEND was added to glibc on 2004-01-15. Reject older versions. */ if (! REG_STARTEND) result |= 64; #if 0 /* It would be nice to reject hosts whose regoff_t values are too narrow (including glibc on hosts with 64-bit ptrdiff_t and 32-bit int), but we should wait until glibc implements this feature. Otherwise, support for equivalence classes and multibyte collation symbols would always be broken except when compiling --without-included-regex. */ if (sizeof (regoff_t) < sizeof (ptrdiff_t) || sizeof (regoff_t) < sizeof (ssize_t)) result |= 64; #endif return result; } gnuastro-0.5/bootstrapped/tests/test-rawmemchr.c0000644000175000017500000000475513217200024017121 00000000000000/* * Copyright (C) 2008-2017 Free Software Foundation, Inc. * Written by Eric Blake and Bruno Haible * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (rawmemchr, void *, (void const *, int)); #include #include "zerosize-ptr.h" #include "macros.h" /* Calculating void * + int is not portable, so this wrapper converts to char * to make the tests easier to write. */ #define RAWMEMCHR (char *) rawmemchr int main (void) { size_t n = 0x100000; char *input = malloc (n + 1); ASSERT (input); input[0] = 'a'; input[1] = 'b'; memset (input + 2, 'c', 1024); memset (input + 1026, 'd', n - 1028); input[n - 2] = 'e'; input[n - 1] = 'a'; input[n] = '\0'; /* Basic behavior tests. */ ASSERT (RAWMEMCHR (input, 'a') == input); ASSERT (RAWMEMCHR (input, 'b') == input + 1); ASSERT (RAWMEMCHR (input, 'c') == input + 2); ASSERT (RAWMEMCHR (input, 'd') == input + 1026); ASSERT (RAWMEMCHR (input + 1, 'a') == input + n - 1); ASSERT (RAWMEMCHR (input + 1, 'e') == input + n - 2); ASSERT (RAWMEMCHR (input + 1, 0x789abc00 | 'e') == input + n - 2); ASSERT (RAWMEMCHR (input, '\0') == input + n); /* Alignment tests. */ { int i, j; for (i = 0; i < 32; i++) { for (j = 0; j < 256; j++) input[i + j] = j; for (j = 0; j < 256; j++) { ASSERT (RAWMEMCHR (input + i, j) == input + i + j); } } } /* Ensure that no unaligned oversized reads occur. */ { char *page_boundary = (char *) zerosize_ptr (); size_t i; if (!page_boundary) page_boundary = input + 4096; memset (page_boundary - 512, '1', 511); page_boundary[-1] = '2'; for (i = 1; i <= 512; i++) ASSERT (RAWMEMCHR (page_boundary - i, (i * 0x01010100) | '2') == page_boundary - 1); } free (input); return 0; } gnuastro-0.5/bootstrapped/tests/test-raise.c0000644000175000017500000000264113217200024016227 00000000000000/* Test raising a signal. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (raise, int, (int)); #include #include "macros.h" /* It is safe to use _Noreturn here: exit() never returns, and GCC knows that exit() is a non-returning function, even on platforms where its declaration in does not have the 'noreturn' attribute. */ static _Noreturn void handler (int sig) { exit (0); } int main (void) { /* Test behaviour for invalid argument. */ ASSERT (raise (-1) != 0); /* Test behaviour for SIGINT. */ ASSERT (signal (SIGINT, handler) != SIG_ERR); raise (SIGINT); /* We should not get here, because the handler takes away the control. */ exit (1); } gnuastro-0.5/bootstrapped/tests/test-pthread_sigmask2.c0000644000175000017500000000453413217200024020356 00000000000000/* Test of pthread_sigmask in a multi-threaded program. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include #include #include #include #include "glthread/thread.h" #include "macros.h" #if USE_POSIX_THREADS static gl_thread_t main_thread; static gl_thread_t killer_thread; static void * killer_thread_func (void *arg) { sleep (1); pthread_kill (main_thread, SIGINT); return NULL; } static volatile int sigint_occurred; static void sigint_handler (int sig) { sigint_occurred++; } int main (int argc, char *argv[]) { sigset_t set; signal (SIGINT, sigint_handler); sigemptyset (&set); sigaddset (&set, SIGINT); /* Check error handling. */ ASSERT (pthread_sigmask (1729, &set, NULL) == EINVAL); /* Block SIGINT. */ ASSERT (pthread_sigmask (SIG_BLOCK, &set, NULL) == 0); /* Request a SIGINT signal from another thread. */ main_thread = gl_thread_self (); ASSERT (glthread_create (&killer_thread, killer_thread_func, NULL) == 0); /* Wait. */ sleep (2); /* The signal should not have arrived yet, because it is blocked. */ ASSERT (sigint_occurred == 0); /* Unblock SIGINT. */ ASSERT (pthread_sigmask (SIG_UNBLOCK, &set, NULL) == 0); /* The signal should have arrived now, because POSIX says "If there are any pending unblocked signals after the call to pthread_sigmask(), at least one of those signals shall be delivered before the call to pthread_sigmask() returns." */ ASSERT (sigint_occurred == 1); return 0; } #else int main () { fputs ("Skipping test: POSIX threads not enabled\n", stderr); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-pthread_sigmask1.c0000644000175000017500000000472513217200024020357 00000000000000/* Test of pthread_sigmask in a single-threaded program. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include #include "signature.h" SIGNATURE_CHECK (pthread_sigmask, int, (int, const sigset_t *, sigset_t *)); #include #include #include #include #include "macros.h" #if !((defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__) static volatile int sigint_occurred; static void sigint_handler (int sig) { sigint_occurred++; } int main (int argc, char *argv[]) { sigset_t set; int pid = getpid (); char command[80]; signal (SIGINT, sigint_handler); sigemptyset (&set); sigaddset (&set, SIGINT); /* Check error handling. */ ASSERT (pthread_sigmask (1729, &set, NULL) == EINVAL); /* Block SIGINT. */ ASSERT (pthread_sigmask (SIG_BLOCK, &set, NULL) == 0); /* Request a SIGINT signal from outside. */ sprintf (command, "sh -c 'sleep 1; kill -%d %d' &", SIGINT, pid); ASSERT (system (command) == 0); /* Wait. */ sleep (2); /* The signal should not have arrived yet, because it is blocked. */ ASSERT (sigint_occurred == 0); /* Unblock SIGINT. */ ASSERT (pthread_sigmask (SIG_UNBLOCK, &set, NULL) == 0); /* The signal should have arrived now, because POSIX says "If there are any pending unblocked signals after the call to pthread_sigmask(), at least one of those signals shall be delivered before the call to pthread_sigmask() returns." */ ASSERT (sigint_occurred == 1); return 0; } #else /* On native Windows, getpid() values and the arguments that are passed to the (Cygwin?) 'kill' program are not necessarily related. */ int main () { fputs ("Skipping test: native Windows platform\n", stderr); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-pipe.c0000644000175000017500000000537713217200024016072 00000000000000/* Test of pipe. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (pipe, int, (int[2])); #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif #endif #include "binary-io.h" #include "macros.h" /* Return true if FD is open. */ static bool is_open (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ return (HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE; #else # ifndef F_GETFL # error Please port fcntl to your platform # endif return 0 <= fcntl (fd, F_GETFL); #endif } /* Return true if FD is not inherited to child processes. */ static bool is_cloexec (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ HANDLE h = (HANDLE) _get_osfhandle (fd); DWORD flags; ASSERT (GetHandleInformation (h, &flags)); return (flags & HANDLE_FLAG_INHERIT) == 0; #else int flags; ASSERT ((flags = fcntl (fd, F_GETFD)) >= 0); return (flags & FD_CLOEXEC) != 0; #endif } /* Return true if FD is in non-blocking mode. */ static bool is_nonblocking (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* We don't use the non-blocking mode for sockets here. */ return 0; #else int flags; ASSERT ((flags = fcntl (fd, F_GETFL)) >= 0); return (flags & O_NONBLOCK) != 0; #endif } int main () { int fd[2]; fd[0] = -1; fd[1] = -1; ASSERT (pipe (fd) >= 0); ASSERT (fd[0] >= 0); ASSERT (fd[1] >= 0); ASSERT (fd[0] != fd[1]); ASSERT (is_open (fd[0])); ASSERT (is_open (fd[1])); ASSERT (!is_cloexec (fd[0])); ASSERT (!is_cloexec (fd[1])); ASSERT (!is_nonblocking (fd[0])); ASSERT (!is_nonblocking (fd[1])); return 0; } gnuastro-0.5/bootstrapped/tests/test-perror2.c0000644000175000017500000000675613217200024016532 00000000000000/* Test of perror() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include #include #include /* This test intentionally parses stderr. So, we arrange to have fd 10 (outside the range of interesting fd's during the test) set up to duplicate the original stderr. */ #define BACKUP_STDERR_FILENO 10 #define ASSERT_STREAM myerr #include "macros.h" static FILE *myerr; #define BASE "test-perror2" int main (void) { /* We change fd 2 later, so save it in fd 10. */ if (dup2 (STDERR_FILENO, BACKUP_STDERR_FILENO) != BACKUP_STDERR_FILENO || (myerr = fdopen (BACKUP_STDERR_FILENO, "w")) == NULL) return 2; ASSERT (freopen (BASE ".tmp", "w+", stderr) == stderr); /* Test that perror does not clobber strerror buffer. */ { const char *msg1; const char *msg2; const char *msg3; const char *msg4; char *str1; char *str2; char *str3; char *str4; msg1 = strerror (ENOENT); ASSERT (msg1); str1 = strdup (msg1); ASSERT (str1); msg2 = strerror (ERANGE); ASSERT (msg2); str2 = strdup (msg2); ASSERT (str2); msg3 = strerror (-4); ASSERT (msg3); str3 = strdup (msg3); ASSERT (str3); msg4 = strerror (1729576); ASSERT (msg4); str4 = strdup (msg4); ASSERT (str4); errno = EACCES; perror (""); errno = -5; perror (""); ASSERT (!ferror (stderr)); ASSERT (msg1 == msg2 || msg1 == msg4 || STREQ (msg1, str1)); ASSERT (msg2 == msg4 || STREQ (msg2, str2)); ASSERT (msg3 == msg4 || STREQ (msg3, str3)); ASSERT (STREQ (msg4, str4)); free (str1); free (str2); free (str3); free (str4); } /* Test that perror uses the same message as strerror. */ { int errs[] = { EACCES, 0, -3, }; int i; for (i = 0; i < SIZEOF (errs); i++) { char buf[256]; char *err = strerror (errs[i]); ASSERT (err); ASSERT (strlen (err) < sizeof buf); rewind (stderr); ASSERT (ftruncate (fileno (stderr), 0) == 0); errno = errs[i]; perror (NULL); ASSERT (!ferror (stderr)); rewind (stderr); ASSERT (fgets (buf, sizeof buf, stderr) == buf); ASSERT (strstr (buf, err)); } } /* Test that perror reports write failure. */ { ASSERT (freopen (BASE ".tmp", "r", stderr) == stderr); ASSERT (setvbuf (stderr, NULL, _IONBF, BUFSIZ) == 0); errno = -1; ASSERT (!ferror (stderr)); perror (NULL); #if 0 /* Commented out until cygwin behaves: https://sourceware.org/ml/newlib/2011/msg00228.html */ ASSERT (errno > 0); /* Commented out until glibc behaves: https://sourceware.org/bugzilla/show_bug.cgi?id=12792 */ ASSERT (ferror (stderr)); #endif } ASSERT (fclose (stderr) == 0); ASSERT (remove (BASE ".tmp") == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-perror.c0000644000175000017500000000205713217200024016436 00000000000000/* Test of perror() function. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (perror, void, (char const *)); #include int main (int argc, char **argv) { const char *prefix = (argc > 1 ? argv[1] : NULL); errno = EACCES; perror (prefix); errno = ETIMEDOUT; perror (prefix); errno = EOVERFLOW; perror (prefix); return 0; } gnuastro-0.5/bootstrapped/tests/test-pathmax.c0000644000175000017500000000170413217200024016565 00000000000000/* Test of "pathmax.h". Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include "pathmax.h" /* Check that PATH_MAX is a constant if it is defined. */ #ifdef PATH_MAX int a = PATH_MAX; #endif int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-open.c0000644000175000017500000000215013217200024016060 00000000000000/* Test of opening a file descriptor. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (open, int, (char const *, int, ...)); #include #include #include #include #include "macros.h" #define BASE "test-open.t" #include "test-open.h" int main (void) { return test_open (open, true); } gnuastro-0.5/bootstrapped/tests/test-nl_langinfo.c0000644000175000017500000001110113217200024017401 00000000000000/* Test of nl_langinfo replacement. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (nl_langinfo, char *, (nl_item)); #include #include #include #include "c-strcase.h" #include "macros.h" /* For GCC >= 4.3, silence the warnings "comparison of unsigned expression >= 0 is always true" in this file. */ #if __GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 3) # pragma GCC diagnostic ignored "-Wtype-limits" #endif int main (int argc, char *argv[]) { int pass = atoi (argv[1]); /* pass locale 0 C 1 traditional French locale 2 French UTF-8 locale */ setlocale (LC_ALL, ""); /* nl_langinfo items of the LC_CTYPE category */ ASSERT (strlen (nl_langinfo (CODESET)) > 0); if (pass == 2) { const char *codeset = nl_langinfo (CODESET); ASSERT (c_strcasecmp (codeset, "UTF-8") == 0 || c_strcasecmp (codeset, "UTF8") == 0); } /* nl_langinfo items of the LC_NUMERIC category */ ASSERT (strlen (nl_langinfo (RADIXCHAR)) > 0); ASSERT (strlen (nl_langinfo (THOUSEP)) >= 0); /* nl_langinfo items of the LC_TIME category */ ASSERT (strlen (nl_langinfo (D_T_FMT)) > 0); ASSERT (strlen (nl_langinfo (D_FMT)) > 0); ASSERT (strlen (nl_langinfo (T_FMT)) > 0); ASSERT (strlen (nl_langinfo (T_FMT_AMPM)) >= (pass == 0 ? 1 : 0)); ASSERT (strlen (nl_langinfo (AM_STR)) >= (pass == 0 ? 1 : 0)); ASSERT (strlen (nl_langinfo (PM_STR)) >= (pass == 0 ? 1 : 0)); ASSERT (strlen (nl_langinfo (DAY_1)) > 0); ASSERT (strlen (nl_langinfo (DAY_2)) > 0); ASSERT (strlen (nl_langinfo (DAY_3)) > 0); ASSERT (strlen (nl_langinfo (DAY_4)) > 0); ASSERT (strlen (nl_langinfo (DAY_5)) > 0); ASSERT (strlen (nl_langinfo (DAY_6)) > 0); ASSERT (strlen (nl_langinfo (DAY_7)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_1)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_2)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_3)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_4)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_5)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_6)) > 0); ASSERT (strlen (nl_langinfo (ABDAY_7)) > 0); ASSERT (strlen (nl_langinfo (MON_1)) > 0); ASSERT (strlen (nl_langinfo (MON_2)) > 0); ASSERT (strlen (nl_langinfo (MON_3)) > 0); ASSERT (strlen (nl_langinfo (MON_4)) > 0); ASSERT (strlen (nl_langinfo (MON_5)) > 0); ASSERT (strlen (nl_langinfo (MON_6)) > 0); ASSERT (strlen (nl_langinfo (MON_7)) > 0); ASSERT (strlen (nl_langinfo (MON_8)) > 0); ASSERT (strlen (nl_langinfo (MON_9)) > 0); ASSERT (strlen (nl_langinfo (MON_10)) > 0); ASSERT (strlen (nl_langinfo (MON_11)) > 0); ASSERT (strlen (nl_langinfo (MON_12)) > 0); ASSERT (strlen (nl_langinfo (ABMON_1)) > 0); ASSERT (strlen (nl_langinfo (ABMON_2)) > 0); ASSERT (strlen (nl_langinfo (ABMON_3)) > 0); ASSERT (strlen (nl_langinfo (ABMON_4)) > 0); ASSERT (strlen (nl_langinfo (ABMON_5)) > 0); ASSERT (strlen (nl_langinfo (ABMON_6)) > 0); ASSERT (strlen (nl_langinfo (ABMON_7)) > 0); ASSERT (strlen (nl_langinfo (ABMON_8)) > 0); ASSERT (strlen (nl_langinfo (ABMON_9)) > 0); ASSERT (strlen (nl_langinfo (ABMON_10)) > 0); ASSERT (strlen (nl_langinfo (ABMON_11)) > 0); ASSERT (strlen (nl_langinfo (ABMON_12)) > 0); ASSERT (strlen (nl_langinfo (ERA)) >= 0); ASSERT (strlen (nl_langinfo (ERA_D_FMT)) >= 0); ASSERT (strlen (nl_langinfo (ERA_D_T_FMT)) >= 0); ASSERT (strlen (nl_langinfo (ERA_T_FMT)) >= 0); ASSERT (nl_langinfo (ALT_DIGITS) != NULL); /* nl_langinfo items of the LC_MONETARY category */ { const char *currency = nl_langinfo (CRNCYSTR); ASSERT (strlen (currency) >= 0); #if !defined __NetBSD__ if (pass > 0) ASSERT (strlen (currency) >= 1); #endif } /* nl_langinfo items of the LC_MESSAGES category */ ASSERT (strlen (nl_langinfo (YESEXPR)) > 0); ASSERT (strlen (nl_langinfo (NOEXPR)) > 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-netinet_in.c0000644000175000017500000000156613217200024017265 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-nanosleep.c0000644000175000017500000000426313217200024017112 00000000000000/* Test of nanosleep() function. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (nanosleep, int, (struct timespec const *, struct timespec *)); #include #include #include #include "macros.h" #if HAVE_DECL_ALARM static void handle_alarm (int sig) { if (sig != SIGALRM) _exit (1); } #endif int main (void) { struct timespec ts; ts.tv_sec = 1000; ts.tv_nsec = -1; errno = 0; ASSERT (nanosleep (&ts, NULL) == -1); ASSERT (errno == EINVAL); ts.tv_nsec = 1000000000; errno = 0; ASSERT (nanosleep (&ts, NULL) == -1); ASSERT (errno == EINVAL); ts.tv_sec = 0; ts.tv_nsec = 1; ASSERT (nanosleep (&ts, &ts) == 0); /* Remaining time is only defined on EINTR failure; but on success, it is typically either 0 or unchanged from input. At any rate, it shouldn't be randomly changed to unrelated values. */ ASSERT (ts.tv_sec == 0); ASSERT (ts.tv_nsec == 0 || ts.tv_nsec == 1); ts.tv_nsec = 0; ASSERT (nanosleep (&ts, NULL) == 0); #if HAVE_DECL_ALARM { const time_t pentecost = 50 * 24 * 60 * 60; /* 50 days. */ signal (SIGALRM, handle_alarm); alarm (1); ts.tv_sec = pentecost; ts.tv_nsec = 999999999; errno = 0; ASSERT (nanosleep (&ts, &ts) == -1); ASSERT (errno == EINTR); ASSERT (pentecost - 10 < ts.tv_sec && ts.tv_sec <= pentecost); ASSERT (0 <= ts.tv_nsec && ts.tv_nsec <= 999999999); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-memchr.c0000644000175000017500000000731313217200024016400 00000000000000/* * Copyright (C) 2008-2017 Free Software Foundation, Inc. * Written by Eric Blake and Bruno Haible * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (memchr, void *, (void const *, int, size_t)); #include #include "zerosize-ptr.h" #include "macros.h" /* Calculating void * + int is not portable, so this wrapper converts to char * to make the tests easier to write. */ #define MEMCHR (char *) memchr int main (void) { size_t n = 0x100000; char *input = malloc (n); ASSERT (input); input[0] = 'a'; input[1] = 'b'; memset (input + 2, 'c', 1024); memset (input + 1026, 'd', n - 1028); input[n - 2] = 'e'; input[n - 1] = 'a'; /* Basic behavior tests. */ ASSERT (MEMCHR (input, 'a', n) == input); ASSERT (MEMCHR (input, 'a', 0) == NULL); ASSERT (MEMCHR (zerosize_ptr (), 'a', 0) == NULL); ASSERT (MEMCHR (input, 'b', n) == input + 1); ASSERT (MEMCHR (input, 'c', n) == input + 2); ASSERT (MEMCHR (input, 'd', n) == input + 1026); ASSERT (MEMCHR (input + 1, 'a', n - 1) == input + n - 1); ASSERT (MEMCHR (input + 1, 'e', n - 1) == input + n - 2); ASSERT (MEMCHR (input + 1, 0x789abc00 | 'e', n - 1) == input + n - 2); ASSERT (MEMCHR (input, 'f', n) == NULL); ASSERT (MEMCHR (input, '\0', n) == NULL); /* Check that a very long haystack is handled quickly if the byte is found near the beginning. */ { size_t repeat = 10000; for (; repeat > 0; repeat--) { ASSERT (MEMCHR (input, 'c', n) == input + 2); } } /* Alignment tests. */ { int i, j; for (i = 0; i < 32; i++) { for (j = 0; j < 256; j++) input[i + j] = j; for (j = 0; j < 256; j++) { ASSERT (MEMCHR (input + i, j, 256) == input + i + j); } } } /* Check that memchr() does not read past the first occurrence of the byte being searched. See the Austin Group's clarification . Test both '\0' and something else, since some implementations special-case searching for NUL. */ { char *page_boundary = (char *) zerosize_ptr (); /* Too small, and we miss cache line boundary tests; too large, and the test takes cubically longer to complete. */ int limit = 257; if (page_boundary != NULL) { for (n = 1; n <= limit; n++) { char *mem = page_boundary - n; memset (mem, 'X', n); ASSERT (MEMCHR (mem, 'U', n) == NULL); ASSERT (MEMCHR (mem, 0, n) == NULL); { size_t i; size_t k; for (i = 0; i < n; i++) { mem[i] = 'U'; for (k = i + 1; k < n + limit; k++) ASSERT (MEMCHR (mem, 'U', k) == mem + i); mem[i] = 0; for (k = i + 1; k < n + limit; k++) ASSERT (MEMCHR (mem, 0, k) == mem + i); mem[i] = 'X'; } } } } } free (input); return 0; } gnuastro-0.5/bootstrapped/tests/test-mbsspn.c0000644000175000017500000000351113217200024016423 00000000000000/* Test of searching a string for a character outside a given set of characters. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include #include "macros.h" int main () { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; ASSERT (mbsspn ("Some text", "") == 0); ASSERT (mbsspn ("A long sentence", " ") == 0); ASSERT (mbsspn (" xy", "aei ou") == 2); ASSERT (mbsspn ("eau", "aeiou") == 3); /* The following tests shows how mbsspn() is different from strspn(). */ { const char input[] = "\303\266\303\274"; /* "öü" */ ASSERT (mbsspn (input, "\303\266") == 2); /* "ö" */ ASSERT (mbsspn (input, "\303\244") == 0); /* "ä" */ ASSERT (mbsspn (input, "\303\274\303\266") == 4); /* "üö" */ ASSERT (mbsspn (input, "\303\244\303\274") == 0); /* "äü" */ ASSERT (mbsspn (input, "\303\244\303\266") == 2); /* "äö" */ } { const char input[] = "\303\266\303\274"; /* "öü" */ ASSERT (mbsspn (input, "\303") == 0); /* invalid multibyte sequence */ } return 0; } gnuastro-0.5/bootstrapped/tests/test-mbspbrk.c0000644000175000017500000000323113217200024016560 00000000000000/* Test of searching a string for a character among a given set of characters. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include #include "macros.h" int main () { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; ASSERT (mbspbrk ("Some text", "") == NULL); { const char input[] = "A long sentence"; ASSERT (mbspbrk (input, "aeiou") == input + 3); ASSERT (mbspbrk (input, "iI") == NULL); } /* The following tests shows how mbspbrk() is different from strpbrk(). */ { const char input[] = "B\303\266se B\303\274bchen"; /* "Böse Bübchen" */ ASSERT (mbspbrk (input, "\303\244\303\274") == input + 7); /* "äü" */ } { const char input[] = "B\303\266se B\303\274bchen"; /* "Böse Bübchen" */ ASSERT (mbspbrk (input, "\303") == NULL); /* invalid multibyte sequence */ } return 0; } gnuastro-0.5/bootstrapped/tests/test-mbsinit.c0000644000175000017500000000267713217200024016602 00000000000000/* Test of test for initial conversion state. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (mbsinit, int, (const mbstate_t *)); #include #include "macros.h" int main (int argc, char *argv[]) { static mbstate_t state; ASSERT (mbsinit (NULL)); ASSERT (mbsinit (&state)); if (argc > 1) { static const char input[1] = "\303"; wchar_t wc; size_t ret; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (!mbsinit (&state)); } return 0; } gnuastro-0.5/bootstrapped/tests/test-mbschr.c0000644000175000017500000000404013217200024016375 00000000000000/* Test of searching a string for a character. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include #include "macros.h" int main () { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; /* Tests with a character < 0x30. */ { const char input[] = "\312\276\300\375 \312\276\300\375 \312\276\300\375"; /* "示例 示例 示例" */ const char *result = mbschr (input, ' '); ASSERT (result == input + 4); } { const char input[] = "\312\276\300\375"; /* "示例" */ const char *result = mbschr (input, ' '); ASSERT (result == NULL); } /* Tests with a character >= 0x30. */ { const char input[] = "\272\305123\324\313\320\320\241\243"; /* "å·123è¿è¡Œã€‚" */ const char *result = mbschr (input, '2'); ASSERT (result == input + 3); } /* This test shows how mbschr() is different from strchr(). */ { const char input[] = "\203\062\332\066123\324\313\320\320\241\243"; /* "씋123è¿è¡Œã€‚" */ const char *result = mbschr (input, '2'); ASSERT (result == input + 5); } { const char input[] = "\312\300\275\347\304\343\272\303\243\241"; /* "世界你好ï¼" */ const char *result = mbschr (input, '!'); ASSERT (result == NULL); } return 0; } gnuastro-0.5/bootstrapped/tests/test-mbrtowc-w32.c0000644000175000017500000005422313217200024017215 00000000000000/* Test of conversion of multibyte character to wide character. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include #include #include "macros.h" #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ static int test_one_locale (const char *name, int codepage) { mbstate_t state; wchar_t wc; size_t ret; # if 1 /* Portable code to set the locale. */ { char name_with_codepage[1024]; sprintf (name_with_codepage, "%s.%d", name, codepage); /* Set the locale. */ if (setlocale (LC_ALL, name_with_codepage) == NULL) return 77; } # else /* Hacky way to set a locale.codepage combination that setlocale() refuses to set. */ { /* Codepage of the current locale, set with setlocale(). Not necessarily the same as GetACP(). */ extern __declspec(dllimport) unsigned int __lc_codepage; /* Set the locale. */ if (setlocale (LC_ALL, name) == NULL) return 77; /* Clobber the codepage and MB_CUR_MAX, both set by setlocale(). */ __lc_codepage = codepage; switch (codepage) { case 1252: case 1256: MB_CUR_MAX = 1; break; case 932: case 950: case 936: MB_CUR_MAX = 2; break; case 54936: case 65001: MB_CUR_MAX = 4; break; } /* Test whether the codepage is really available. */ memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, " ", 1, &state) == (size_t)(-1)) return 77; } # endif /* Test zero-length input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "x", 0, &state); /* gnulib's implementation returns (size_t)(-2). The AIX 5.1 implementation returns (size_t)(-1). glibc's implementation returns 0. */ ASSERT (ret == (size_t)(-2) || ret == (size_t)(-1) || ret == 0); ASSERT (mbsinit (&state)); } /* Test NUL byte input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "", 1, &state); ASSERT (ret == 0); ASSERT (wc == 0); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, "", 1, &state); ASSERT (ret == 0); ASSERT (mbsinit (&state)); } /* Test single-byte input. */ { int c; char buf[1]; memset (&state, '\0', sizeof (mbstate_t)); for (c = 0; c < 0x100; c++) switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set". */ buf[0] = c; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, buf, 1, &state); ASSERT (ret == 1); ASSERT (wc == c); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, buf, 1, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); break; } } /* Test special calling convention, passing a NULL pointer. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, NULL, 5, &state); ASSERT (ret == 0); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (mbsinit (&state)); } switch (codepage) { case 1252: /* Locale encoding is CP1252, an extension of ISO-8859-1. */ { char input[] = "B\374\337er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\374'); ASSERT (wc == 0x00FC); ASSERT (mbsinit (&state)); input[1] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\337'); ASSERT (wc == 0x00DF); ASSERT (mbsinit (&state)); input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case 1256: /* Locale encoding is CP1256, not the same as ISO-8859-6. */ { char input[] = "x\302\341\346y"; /* "xآلوy" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'x'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\302'); ASSERT (wc == 0x0622); ASSERT (mbsinit (&state)); input[1] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\341'); ASSERT (wc == 0x0644); ASSERT (mbsinit (&state)); input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 2, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\346'); ASSERT (wc == 0x0648); ASSERT (mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'y'); ASSERT (mbsinit (&state)); } return 0; case 932: /* Locale encoding is CP932, similar to Shift_JIS. */ { char input[] = "<\223\372\226\173\214\352>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x65E5); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x672C); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x8A9E); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT ((ret == (size_t)-1 && errno == EILSEQ) || ret == (size_t)-2); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT ((ret == (size_t)-1 && errno == EILSEQ) || (ret == 2 && wc == 0x30FB)); } return 0; case 950: /* Locale encoding is CP950, similar to Big5. */ { char input[] = "<\244\351\245\273\273\171>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x65E5); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x672C); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x8A9E); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT ((ret == (size_t)-1 && errno == EILSEQ) || ret == (size_t)-2); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT ((ret == (size_t)-1 && errno == EILSEQ) || (ret == 2 && wc == '?')); } return 0; case 936: /* Locale encoding is CP936 = GBK, an extension of GB2312. */ { char input[] = "<\310\325\261\276\325\132>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x65E5); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x672C); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x8A9E); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT ((ret == (size_t)-1 && errno == EILSEQ) || ret == (size_t)-2); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT ((ret == (size_t)-1 && errno == EILSEQ) || (ret == 2 && wc == '?')); } return 0; case 54936: /* Locale encoding is CP54936 = GB18030. */ { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 7, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00FC); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00DF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 8, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\225\377", 2, &state); /* 0x95 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\045", 2, &state); /* 0x81 0x25 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\060\377", 3, &state); /* 0x81 0x30 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\060\377\064", 4, &state); /* 0x81 0x30 0xFF 0x34 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\201\060\211\072", 4, &state); /* 0x81 0x30 0x89 0x3A */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; case 65001: /* Locale encoding is CP65001 = UTF-8. */ { char input[] = "B\303\274\303\237er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 5, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00FC); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (wc == 0x00DF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 6, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); /* Test some invalid input. */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\377", 1, &state); /* 0xFF */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\303\300", 2, &state); /* 0xC3 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\343\300", 2, &state); /* 0xE3 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\343\300\200", 3, &state); /* 0xE3 0xC0 0x80 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\343\200\300", 3, &state); /* 0xE3 0x80 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\300", 2, &state); /* 0xF3 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\300\200\200", 4, &state); /* 0xF3 0xC0 0x80 0x80 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\200\300", 3, &state); /* 0xF3 0x80 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\200\300\200", 4, &state); /* 0xF3 0x80 0xC0 0x80 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "\363\200\200\300", 4, &state); /* 0xF3 0x80 0x80 0xC0 */ ASSERT (ret == (size_t)-1); ASSERT (errno == EILSEQ); } return 0; default: return 1; } } int main (int argc, char *argv[]) { int codepage = atoi (argv[argc - 1]); int result; int i; result = 77; for (i = 1; i < argc - 1; i++) { int ret = test_one_locale (argv[i], codepage); if (ret != 77) result = ret; } if (result == 77) { fprintf (stderr, "Skipping test: found no locale with codepage %d\n", codepage); } return result; } #else int main (int argc, char *argv[]) { fputs ("Skipping test: not a native Windows system\n", stderr); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-mbrtowc.c0000644000175000017500000002521713217200024016605 00000000000000/* Test of conversion of multibyte character to wide character. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (mbrtowc, size_t, (wchar_t *, char const *, size_t, mbstate_t *)); #include #include #include #include "macros.h" int main (int argc, char *argv[]) { mbstate_t state; wchar_t wc; size_t ret; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; /* Test zero-length input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "x", 0, &state); ASSERT (ret == (size_t)(-2)); ASSERT (mbsinit (&state)); } /* Test NUL byte input. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, "", 1, &state); ASSERT (ret == 0); ASSERT (wc == 0); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, "", 1, &state); ASSERT (ret == 0); ASSERT (mbsinit (&state)); } /* Test single-byte input. */ { int c; char buf[1]; memset (&state, '\0', sizeof (mbstate_t)); for (c = 0; c < 0x100; c++) switch (c) { default: if (! (c && 1 < argc && argv[1][0] == '5')) break; FALLTHROUGH; case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': /* c is in the ISO C "basic character set", or argv[1] starts with '5' so we are testing all nonnull bytes. */ buf[0] = c; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, buf, 1, &state); ASSERT (ret == 1); ASSERT (wc == c); ASSERT (mbsinit (&state)); ret = mbrtowc (NULL, buf, 1, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); break; } } /* Test special calling convention, passing a NULL pointer. */ { memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, NULL, 5, &state); ASSERT (ret == 0); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (mbsinit (&state)); } if (argc > 1) switch (argv[1][0]) { case '1': /* Locale encoding is ISO-8859-1 or ISO-8859-15. */ { char input[] = "B\374\337er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\374'); ASSERT (mbsinit (&state)); input[1] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 3, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == (unsigned char) '\337'); ASSERT (mbsinit (&state)); input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case '2': /* Locale encoding is UTF-8. */ { char input[] = "B\303\274\303\237er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 5, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 4, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 6, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case '3': /* Locale encoding is EUC-JP. */ { char input[] = "<\306\374\313\334\270\354>"; /* "<日本語>" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == '<'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 2, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[1] = '\0'; input[2] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[3] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 4, 4, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[4] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 5, 3, &state); ASSERT (ret == 2); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 1, &state); ASSERT (ret == 1); ASSERT (wc == '>'); ASSERT (mbsinit (&state)); } return 0; case '4': /* Locale encoding is GB18030. */ { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'B'); ASSERT (mbsinit (&state)); input[0] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 1, 1, &state); ASSERT (ret == (size_t)(-2)); ASSERT (wc == (wchar_t) 0xBADFACE); ASSERT (!mbsinit (&state)); input[1] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 2, 7, &state); ASSERT (ret == 1); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[2] = '\0'; /* Test support of NULL first argument. */ ret = mbrtowc (NULL, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (mbsinit (&state)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 3, 6, &state); ASSERT (ret == 4); ASSERT (wctob (wc) == EOF); ASSERT (mbsinit (&state)); input[3] = '\0'; input[4] = '\0'; input[5] = '\0'; input[6] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 7, 2, &state); ASSERT (ret == 1); ASSERT (wc == 'e'); ASSERT (mbsinit (&state)); input[5] = '\0'; wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input + 8, 1, &state); ASSERT (ret == 1); ASSERT (wc == 'r'); ASSERT (mbsinit (&state)); } return 0; case '5': /* C locale; tested above. */ return 0; } return 1; } gnuastro-0.5/bootstrapped/tests/test-math.c0000644000175000017500000000435113217200024016055 00000000000000/* Test of substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #ifndef NAN # error NAN should be defined choke me #endif #ifndef HUGE_VALF # error HUGE_VALF should be defined choke me #endif #ifndef HUGE_VAL # error HUGE_VAL should be defined choke me #endif #ifndef HUGE_VALL # error HUGE_VALL should be defined choke me #endif #ifndef FP_ILOGB0 # error FP_ILOGB0 should be defined choke me #endif #ifndef FP_ILOGBNAN # error FP_ILOGBNAN should be defined choke me #endif #include #include "macros.h" #if 0 /* Check that NAN expands into a constant expression. */ static float n = NAN; #endif /* Compare two numbers with ==. This is a separate function because IRIX 6.5 "cc -O" miscompiles an 'x == x' test. */ static int numeric_equalf (float x, float y) { return x == y; } static int numeric_equald (double x, double y) { return x == y; } static int numeric_equall (long double x, long double y) { return x == y; } int main (void) { double d = NAN; double zero = 0.0; ASSERT (!numeric_equald (d, d)); d = HUGE_VAL; ASSERT (numeric_equald (d, 1.0 / zero)); ASSERT (numeric_equalf (HUGE_VALF, HUGE_VALF + HUGE_VALF)); ASSERT (numeric_equald (HUGE_VAL, HUGE_VAL + HUGE_VAL)); ASSERT (numeric_equall (HUGE_VALL, HUGE_VALL + HUGE_VALL)); /* Check the value of FP_ILOGB0. */ ASSERT (FP_ILOGB0 == INT_MIN || FP_ILOGB0 == - INT_MAX); /* Check the value of FP_ILOGBNAN. */ ASSERT (FP_ILOGBNAN == INT_MIN || FP_ILOGBNAN == INT_MAX); return 0; } gnuastro-0.5/bootstrapped/tests/test-malloca.c0000644000175000017500000000306113217200024016531 00000000000000/* Test of safe automatic memory allocation. Copyright (C) 2005, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #include "malloca.h" #include static void do_allocation (int n) { void *ptr = malloca (n); freea (ptr); safe_alloca (n); } void (*func) (int) = do_allocation; int main () { int i; /* This slows down malloc a lot. */ unsetenv ("MALLOC_PERTURB_"); /* Repeat a lot of times, to make sure there's no memory leak. */ for (i = 0; i < 50000; i++) { /* Try various values. n = 0 gave a crash on Alpha with gcc-2.5.8. Some versions of Mac OS X have a stack size limit of 512 KB. */ func (34); func (134); func (399); func (510823); func (129321); func (0); func (4070); func (4095); func (1); func (16582); } return 0; } gnuastro-0.5/bootstrapped/tests/test-malloc-gnu.c0000644000175000017500000000163713217200024017166 00000000000000/* Test of malloc function. Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include int main () { /* Check that malloc (0) is not a NULL pointer. */ char *p = malloc (0); if (p == NULL) return 1; free (p); return 0; } gnuastro-0.5/bootstrapped/tests/test-lstat.c0000644000175000017500000000340613217200024016253 00000000000000/* Test of lstat() function. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson, 2008; and Eric Blake, 2009. */ #include #include /* Caution: lstat may be a function-like macro. Although this signature check must pass, it may be the signature of the real (and broken) lstat rather than rpl_lstat. Most code should not use the address of lstat. */ #include "signature.h" SIGNATURE_CHECK (lstat, int, (char const *, struct stat *)); #include #include #include #include #include #include #include "same-inode.h" #include "ignore-value.h" #include "macros.h" #define BASE "test-lstat.t" #include "test-lstat.h" /* Wrapper around lstat, which works even if lstat is a function-like macro, where test_lstat_func(lstat) would do the wrong thing. */ static int do_lstat (char const *name, struct stat *st) { return lstat (name, st); } int main (void) { /* Remove any leftovers from a previous partial run. */ ignore_value (system ("rm -rf " BASE "*")); return test_lstat_func (do_lstat, true); } gnuastro-0.5/bootstrapped/tests/test-lock.c0000644000175000017500000004675713217200024016074 00000000000000/* Test of locking in multithreaded situations. Copyright (C) 2005, 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #if USE_POSIX_THREADS || USE_SOLARIS_THREADS || USE_PTH_THREADS || USE_WINDOWS_THREADS #if USE_POSIX_THREADS # define TEST_POSIX_THREADS 1 #endif #if USE_SOLARIS_THREADS # define TEST_SOLARIS_THREADS 1 #endif #if USE_PTH_THREADS # define TEST_PTH_THREADS 1 #endif #if USE_WINDOWS_THREADS # define TEST_WINDOWS_THREADS 1 #endif /* Whether to enable locking. Uncomment this to get a test program without locking, to verify that it crashes. */ #define ENABLE_LOCKING 1 /* Which tests to perform. Uncomment some of these, to verify that all tests crash if no locking is enabled. */ #define DO_TEST_LOCK 1 #define DO_TEST_RWLOCK 1 #define DO_TEST_RECURSIVE_LOCK 1 #define DO_TEST_ONCE 1 /* Whether to help the scheduler through explicit yield(). Uncomment this to see if the operating system has a fair scheduler. */ #define EXPLICIT_YIELD 1 /* Whether to use 'volatile' on some variables that communicate information between threads. If set to 0, a semaphore or a lock is used to protect these variables. If set to 1, 'volatile' is used; this is theoretically equivalent but can lead to much slower execution (e.g. 30x slower total run time on a 40-core machine), because 'volatile' does not imply any synchronization/communication between different CPUs. */ #define USE_VOLATILE 0 #if USE_POSIX_THREADS && HAVE_SEMAPHORE_H /* Whether to use a semaphore to communicate information between threads. If set to 0, a lock is used. If set to 1, a semaphore is used. Uncomment this to reduce the dependencies of this test. */ # define USE_SEMAPHORE 1 /* Mac OS X provides only named semaphores (sem_open); its facility for unnamed semaphores (sem_init) does not work. */ # if defined __APPLE__ && defined __MACH__ # define USE_NAMED_SEMAPHORE 1 # else # define USE_UNNAMED_SEMAPHORE 1 # endif #endif /* Whether to print debugging messages. */ #define ENABLE_DEBUGGING 0 /* Number of simultaneous threads. */ #define THREAD_COUNT 10 /* Number of operations performed in each thread. This is quite high, because with a smaller count, say 5000, we often get an "OK" result even without ENABLE_LOCKING (on Linux/x86). */ #define REPEAT_COUNT 50000 #include #include #include #if !ENABLE_LOCKING # undef USE_POSIX_THREADS # undef USE_SOLARIS_THREADS # undef USE_PTH_THREADS # undef USE_WINDOWS_THREADS #endif #include "glthread/lock.h" #if !ENABLE_LOCKING # if TEST_POSIX_THREADS # define USE_POSIX_THREADS 1 # endif # if TEST_SOLARIS_THREADS # define USE_SOLARIS_THREADS 1 # endif # if TEST_PTH_THREADS # define USE_PTH_THREADS 1 # endif # if TEST_WINDOWS_THREADS # define USE_WINDOWS_THREADS 1 # endif #endif #include "glthread/thread.h" #include "glthread/yield.h" #if USE_SEMAPHORE # include # include # include # include #endif #if ENABLE_DEBUGGING # define dbgprintf printf #else # define dbgprintf if (0) printf #endif #if EXPLICIT_YIELD # define yield() gl_thread_yield () #else # define yield() #endif #if USE_VOLATILE struct atomic_int { volatile int value; }; static void init_atomic_int (struct atomic_int *ai) { } static int get_atomic_int_value (struct atomic_int *ai) { return ai->value; } static void set_atomic_int_value (struct atomic_int *ai, int new_value) { ai->value = new_value; } #elif USE_SEMAPHORE /* This atomic_int implementation can only support the values 0 and 1. It is initially 0 and can be set to 1 only once. */ # if USE_UNNAMED_SEMAPHORE struct atomic_int { sem_t semaphore; }; #define atomic_int_semaphore(ai) (&(ai)->semaphore) static void init_atomic_int (struct atomic_int *ai) { sem_init (&ai->semaphore, 0, 0); } # endif # if USE_NAMED_SEMAPHORE struct atomic_int { sem_t *semaphore; }; #define atomic_int_semaphore(ai) ((ai)->semaphore) static void init_atomic_int (struct atomic_int *ai) { sem_t *s; unsigned int count; for (count = 0; ; count++) { char name[80]; /* Use getpid() in the name, so that different processes running at the same time will not interfere. Use ai in the name, so that different atomic_int in the same process will not interfere. Use a count in the name, so that even in the (unlikely) case that a semaphore with the specified name already exists, we can try a different name. */ sprintf (name, "test-lock-%lu-%p-%u", (unsigned long) getpid (), ai, count); s = sem_open (name, O_CREAT | O_EXCL, 0600, 0); if (s == SEM_FAILED) { if (errno == EEXIST) /* Retry with a different name. */ continue; else { perror ("sem_open failed"); abort (); } } else { /* Try not to leave a semaphore hanging around on the file system eternally, if we can avoid it. */ sem_unlink (name); break; } } ai->semaphore = s; } # endif static int get_atomic_int_value (struct atomic_int *ai) { if (sem_trywait (atomic_int_semaphore (ai)) == 0) { if (sem_post (atomic_int_semaphore (ai))) abort (); return 1; } else if (errno == EAGAIN) return 0; else abort (); } static void set_atomic_int_value (struct atomic_int *ai, int new_value) { if (new_value == 0) /* It's already initialized with 0. */ return; /* To set the value 1: */ if (sem_post (atomic_int_semaphore (ai))) abort (); } #else struct atomic_int { gl_lock_define (, lock) int value; }; static void init_atomic_int (struct atomic_int *ai) { gl_lock_init (ai->lock); } static int get_atomic_int_value (struct atomic_int *ai) { gl_lock_lock (ai->lock); int ret = ai->value; gl_lock_unlock (ai->lock); return ret; } static void set_atomic_int_value (struct atomic_int *ai, int new_value) { gl_lock_lock (ai->lock); ai->value = new_value; gl_lock_unlock (ai->lock); } #endif #define ACCOUNT_COUNT 4 static int account[ACCOUNT_COUNT]; static int random_account (void) { return ((unsigned int) rand () >> 3) % ACCOUNT_COUNT; } static void check_accounts (void) { int i, sum; sum = 0; for (i = 0; i < ACCOUNT_COUNT; i++) sum += account[i]; if (sum != ACCOUNT_COUNT * 1000) abort (); } /* ------------------- Test normal (non-recursive) locks ------------------- */ /* Test normal locks by having several bank accounts and several threads which shuffle around money between the accounts and another thread checking that all the money is still there. */ gl_lock_define_initialized(static, my_lock) static void * lock_mutator_thread (void *arg) { int repeat; for (repeat = REPEAT_COUNT; repeat > 0; repeat--) { int i1, i2, value; dbgprintf ("Mutator %p before lock\n", gl_thread_self_pointer ()); gl_lock_lock (my_lock); dbgprintf ("Mutator %p after lock\n", gl_thread_self_pointer ()); i1 = random_account (); i2 = random_account (); value = ((unsigned int) rand () >> 3) % 10; account[i1] += value; account[i2] -= value; dbgprintf ("Mutator %p before unlock\n", gl_thread_self_pointer ()); gl_lock_unlock (my_lock); dbgprintf ("Mutator %p after unlock\n", gl_thread_self_pointer ()); dbgprintf ("Mutator %p before check lock\n", gl_thread_self_pointer ()); gl_lock_lock (my_lock); check_accounts (); gl_lock_unlock (my_lock); dbgprintf ("Mutator %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Mutator %p dying.\n", gl_thread_self_pointer ()); return NULL; } static struct atomic_int lock_checker_done; static void * lock_checker_thread (void *arg) { while (get_atomic_int_value (&lock_checker_done) == 0) { dbgprintf ("Checker %p before check lock\n", gl_thread_self_pointer ()); gl_lock_lock (my_lock); check_accounts (); gl_lock_unlock (my_lock); dbgprintf ("Checker %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Checker %p dying.\n", gl_thread_self_pointer ()); return NULL; } static void test_lock (void) { int i; gl_thread_t checkerthread; gl_thread_t threads[THREAD_COUNT]; /* Initialization. */ for (i = 0; i < ACCOUNT_COUNT; i++) account[i] = 1000; init_atomic_int (&lock_checker_done); set_atomic_int_value (&lock_checker_done, 0); /* Spawn the threads. */ checkerthread = gl_thread_create (lock_checker_thread, NULL); for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (lock_mutator_thread, NULL); /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); set_atomic_int_value (&lock_checker_done, 1); gl_thread_join (checkerthread, NULL); check_accounts (); } /* ----------------- Test read-write (non-recursive) locks ----------------- */ /* Test read-write locks by having several bank accounts and several threads which shuffle around money between the accounts and several other threads that check that all the money is still there. */ gl_rwlock_define_initialized(static, my_rwlock) static void * rwlock_mutator_thread (void *arg) { int repeat; for (repeat = REPEAT_COUNT; repeat > 0; repeat--) { int i1, i2, value; dbgprintf ("Mutator %p before wrlock\n", gl_thread_self_pointer ()); gl_rwlock_wrlock (my_rwlock); dbgprintf ("Mutator %p after wrlock\n", gl_thread_self_pointer ()); i1 = random_account (); i2 = random_account (); value = ((unsigned int) rand () >> 3) % 10; account[i1] += value; account[i2] -= value; dbgprintf ("Mutator %p before unlock\n", gl_thread_self_pointer ()); gl_rwlock_unlock (my_rwlock); dbgprintf ("Mutator %p after unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Mutator %p dying.\n", gl_thread_self_pointer ()); return NULL; } static struct atomic_int rwlock_checker_done; static void * rwlock_checker_thread (void *arg) { while (get_atomic_int_value (&rwlock_checker_done) == 0) { dbgprintf ("Checker %p before check rdlock\n", gl_thread_self_pointer ()); gl_rwlock_rdlock (my_rwlock); check_accounts (); gl_rwlock_unlock (my_rwlock); dbgprintf ("Checker %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Checker %p dying.\n", gl_thread_self_pointer ()); return NULL; } static void test_rwlock (void) { int i; gl_thread_t checkerthreads[THREAD_COUNT]; gl_thread_t threads[THREAD_COUNT]; /* Initialization. */ for (i = 0; i < ACCOUNT_COUNT; i++) account[i] = 1000; init_atomic_int (&rwlock_checker_done); set_atomic_int_value (&rwlock_checker_done, 0); /* Spawn the threads. */ for (i = 0; i < THREAD_COUNT; i++) checkerthreads[i] = gl_thread_create (rwlock_checker_thread, NULL); for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (rwlock_mutator_thread, NULL); /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); set_atomic_int_value (&rwlock_checker_done, 1); for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (checkerthreads[i], NULL); check_accounts (); } /* -------------------------- Test recursive locks -------------------------- */ /* Test recursive locks by having several bank accounts and several threads which shuffle around money between the accounts (recursively) and another thread checking that all the money is still there. */ gl_recursive_lock_define_initialized(static, my_reclock) static void recshuffle (void) { int i1, i2, value; dbgprintf ("Mutator %p before lock\n", gl_thread_self_pointer ()); gl_recursive_lock_lock (my_reclock); dbgprintf ("Mutator %p after lock\n", gl_thread_self_pointer ()); i1 = random_account (); i2 = random_account (); value = ((unsigned int) rand () >> 3) % 10; account[i1] += value; account[i2] -= value; /* Recursive with probability 0.5. */ if (((unsigned int) rand () >> 3) % 2) recshuffle (); dbgprintf ("Mutator %p before unlock\n", gl_thread_self_pointer ()); gl_recursive_lock_unlock (my_reclock); dbgprintf ("Mutator %p after unlock\n", gl_thread_self_pointer ()); } static void * reclock_mutator_thread (void *arg) { int repeat; for (repeat = REPEAT_COUNT; repeat > 0; repeat--) { recshuffle (); dbgprintf ("Mutator %p before check lock\n", gl_thread_self_pointer ()); gl_recursive_lock_lock (my_reclock); check_accounts (); gl_recursive_lock_unlock (my_reclock); dbgprintf ("Mutator %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Mutator %p dying.\n", gl_thread_self_pointer ()); return NULL; } static struct atomic_int reclock_checker_done; static void * reclock_checker_thread (void *arg) { while (get_atomic_int_value (&reclock_checker_done) == 0) { dbgprintf ("Checker %p before check lock\n", gl_thread_self_pointer ()); gl_recursive_lock_lock (my_reclock); check_accounts (); gl_recursive_lock_unlock (my_reclock); dbgprintf ("Checker %p after check unlock\n", gl_thread_self_pointer ()); yield (); } dbgprintf ("Checker %p dying.\n", gl_thread_self_pointer ()); return NULL; } static void test_recursive_lock (void) { int i; gl_thread_t checkerthread; gl_thread_t threads[THREAD_COUNT]; /* Initialization. */ for (i = 0; i < ACCOUNT_COUNT; i++) account[i] = 1000; init_atomic_int (&reclock_checker_done); set_atomic_int_value (&reclock_checker_done, 0); /* Spawn the threads. */ checkerthread = gl_thread_create (reclock_checker_thread, NULL); for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (reclock_mutator_thread, NULL); /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); set_atomic_int_value (&reclock_checker_done, 1); gl_thread_join (checkerthread, NULL); check_accounts (); } /* ------------------------ Test once-only execution ------------------------ */ /* Test once-only execution by having several threads attempt to grab a once-only task simultaneously (triggered by releasing a read-write lock). */ gl_once_define(static, fresh_once) static int ready[THREAD_COUNT]; static gl_lock_t ready_lock[THREAD_COUNT]; #if ENABLE_LOCKING static gl_rwlock_t fire_signal[REPEAT_COUNT]; #else static volatile int fire_signal_state; #endif static gl_once_t once_control; static int performed; gl_lock_define_initialized(static, performed_lock) static void once_execute (void) { gl_lock_lock (performed_lock); performed++; gl_lock_unlock (performed_lock); } static void * once_contender_thread (void *arg) { int id = (int) (long) arg; int repeat; for (repeat = 0; repeat <= REPEAT_COUNT; repeat++) { /* Tell the main thread that we're ready. */ gl_lock_lock (ready_lock[id]); ready[id] = 1; gl_lock_unlock (ready_lock[id]); if (repeat == REPEAT_COUNT) break; dbgprintf ("Contender %p waiting for signal for round %d\n", gl_thread_self_pointer (), repeat); #if ENABLE_LOCKING /* Wait for the signal to go. */ gl_rwlock_rdlock (fire_signal[repeat]); /* And don't hinder the others (if the scheduler is unfair). */ gl_rwlock_unlock (fire_signal[repeat]); #else /* Wait for the signal to go. */ while (fire_signal_state <= repeat) yield (); #endif dbgprintf ("Contender %p got the signal for round %d\n", gl_thread_self_pointer (), repeat); /* Contend for execution. */ gl_once (once_control, once_execute); } return NULL; } static void test_once (void) { int i, repeat; gl_thread_t threads[THREAD_COUNT]; /* Initialize all variables. */ for (i = 0; i < THREAD_COUNT; i++) { ready[i] = 0; gl_lock_init (ready_lock[i]); } #if ENABLE_LOCKING for (i = 0; i < REPEAT_COUNT; i++) gl_rwlock_init (fire_signal[i]); #else fire_signal_state = 0; #endif /* Block all fire_signals. */ for (i = REPEAT_COUNT-1; i >= 0; i--) gl_rwlock_wrlock (fire_signal[i]); /* Spawn the threads. */ for (i = 0; i < THREAD_COUNT; i++) threads[i] = gl_thread_create (once_contender_thread, (void *) (long) i); for (repeat = 0; repeat <= REPEAT_COUNT; repeat++) { /* Wait until every thread is ready. */ dbgprintf ("Main thread before synchronizing for round %d\n", repeat); for (;;) { int ready_count = 0; for (i = 0; i < THREAD_COUNT; i++) { gl_lock_lock (ready_lock[i]); ready_count += ready[i]; gl_lock_unlock (ready_lock[i]); } if (ready_count == THREAD_COUNT) break; yield (); } dbgprintf ("Main thread after synchronizing for round %d\n", repeat); if (repeat > 0) { /* Check that exactly one thread executed the once_execute() function. */ if (performed != 1) abort (); } if (repeat == REPEAT_COUNT) break; /* Preparation for the next round: Initialize once_control. */ memcpy (&once_control, &fresh_once, sizeof (gl_once_t)); /* Preparation for the next round: Reset the performed counter. */ performed = 0; /* Preparation for the next round: Reset the ready flags. */ for (i = 0; i < THREAD_COUNT; i++) { gl_lock_lock (ready_lock[i]); ready[i] = 0; gl_lock_unlock (ready_lock[i]); } /* Signal all threads simultaneously. */ dbgprintf ("Main thread giving signal for round %d\n", repeat); #if ENABLE_LOCKING gl_rwlock_unlock (fire_signal[repeat]); #else fire_signal_state = repeat + 1; #endif } /* Wait for the threads to terminate. */ for (i = 0; i < THREAD_COUNT; i++) gl_thread_join (threads[i], NULL); } /* -------------------------------------------------------------------------- */ int main () { #if TEST_PTH_THREADS if (!pth_init ()) abort (); #endif #if DO_TEST_LOCK printf ("Starting test_lock ..."); fflush (stdout); test_lock (); printf (" OK\n"); fflush (stdout); #endif #if DO_TEST_RWLOCK printf ("Starting test_rwlock ..."); fflush (stdout); test_rwlock (); printf (" OK\n"); fflush (stdout); #endif #if DO_TEST_RECURSIVE_LOCK printf ("Starting test_recursive_lock ..."); fflush (stdout); test_recursive_lock (); printf (" OK\n"); fflush (stdout); #endif #if DO_TEST_ONCE printf ("Starting test_once ..."); fflush (stdout); test_once (); printf (" OK\n"); fflush (stdout); #endif return 0; } #else /* No multithreading available. */ #include int main () { fputs ("Skipping test: multithreading not enabled\n", stderr); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-localename.c0000644000175000017500000005472613217200024017237 00000000000000/* Test of gl_locale_name function and its variants. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "localename.h" #include #include #include #include "macros.h" #if HAVE_NEWLOCALE && HAVE_USELOCALE static struct { int cat; int mask; const char *string; } const categories[] = { { LC_CTYPE, LC_CTYPE_MASK, "LC_CTYPE" }, { LC_NUMERIC, LC_NUMERIC_MASK, "LC_NUMERIC" }, { LC_TIME, LC_TIME_MASK, "LC_TIME" }, { LC_COLLATE, LC_COLLATE_MASK, "LC_COLLATE" }, { LC_MONETARY, LC_MONETARY_MASK, "LC_MONETARY" }, { LC_MESSAGES, LC_MESSAGES_MASK, "LC_MESSAGES" } # ifdef LC_PAPER , { LC_PAPER, LC_PAPER_MASK, "LC_PAPER" } # endif # ifdef LC_NAME , { LC_NAME, LC_NAME_MASK, "LC_NAME" } # endif # ifdef LC_ADDRESS , { LC_ADDRESS, LC_ADDRESS_MASK, "LC_ADDRESS" } # endif # ifdef LC_TELEPHONE , { LC_TELEPHONE, LC_TELEPHONE_MASK, "LC_TELEPHONE" } # endif # ifdef LC_MEASUREMENT , { LC_MEASUREMENT, LC_MEASUREMENT_MASK, "LC_MEASUREMENT" } # endif # ifdef LC_IDENTIFICATION , { LC_IDENTIFICATION, LC_IDENTIFICATION_MASK, "LC_IDENTIFICATION" } # endif }; #endif /* Test the gl_locale_name() function. */ static void test_locale_name (void) { const char *name; /* Check that gl_locale_name returns non-NULL. */ ASSERT (gl_locale_name (LC_MESSAGES, "LC_MESSAGES") != NULL); /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE && HAVE_USELOCALE uselocale (LC_GLOBAL_LOCALE); #endif /* Check that when all environment variables are unset, gl_locale_name returns the default locale. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LC_NUMERIC"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); ASSERT (strcmp (gl_locale_name (LC_NUMERIC, "LC_NUMERIC"), gl_locale_name_default ()) == 0); /* Check that an empty environment variable is treated like an unset environment variable. */ setenv ("LC_ALL", "", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "", 1); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "", 1); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), gl_locale_name_default ()) == 0); /* Check that LC_ALL overrides the others, and LANG is overridden by the others. */ setenv ("LC_ALL", "C", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), "C") == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "C", 1); setenv ("LC_MESSAGES", "C", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), "C") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); ASSERT (strcmp (gl_locale_name (LC_MESSAGES, "LC_MESSAGES"), "C") == 0); /* Check mixed situations. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); setenv ("LANG", "de_DE.UTF-8", 1); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "de_DE.UTF-8") == 0); name = gl_locale_name (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); unsetenv ("LANG"); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, gl_locale_name_default ()) == 0); name = gl_locale_name (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } #if HAVE_NEWLOCALE && HAVE_USELOCALE /* Check that gl_locale_name considers the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { uselocale (locale); name = gl_locale_name (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); name = gl_locale_name (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Check that gl_locale_name distinguishes different categories of the thread locale, and that the name is the right one for each. */ { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) { int category_mask = categories[i].mask; locale_t loc = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (loc != NULL) { locale_t locale = newlocale (category_mask, "de_DE.UTF-8", loc); if (locale == NULL) freelocale (loc); else { unsigned int j; uselocale (locale); for (j = 0; j < SIZEOF (categories); j++) { const char *name_j = gl_locale_name (categories[j].cat, categories[j].string); if (j == i) ASSERT (strcmp (name_j, "de_DE.UTF-8") == 0); else ASSERT (strcmp (name_j, "fr_FR.UTF-8") == 0); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } } } #endif } /* Test the gl_locale_name_thread() function. */ static void test_locale_name_thread (void) { /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE && HAVE_USELOCALE /* Check that gl_locale_name_thread returns NULL when no thread locale is set. */ uselocale (LC_GLOBAL_LOCALE); ASSERT (gl_locale_name_thread (LC_CTYPE, "LC_CTYPE") == NULL); ASSERT (gl_locale_name_thread (LC_MESSAGES, "LC_MESSAGES") == NULL); /* Check that gl_locale_name_thread considers the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { const char *name; uselocale (locale); name = gl_locale_name_thread (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); name = gl_locale_name_thread (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Check that gl_locale_name_thread distinguishes different categories of the thread locale, and that the name is the right one for each. */ { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) { int category_mask = categories[i].mask; locale_t loc = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (loc != NULL) { locale_t locale = newlocale (category_mask, "de_DE.UTF-8", loc); if (locale == NULL) freelocale (loc); else { unsigned int j; uselocale (locale); for (j = 0; j < SIZEOF (categories); j++) { const char *name_j = gl_locale_name_thread (categories[j].cat, categories[j].string); if (j == i) ASSERT (strcmp (name_j, "de_DE.UTF-8") == 0); else ASSERT (strcmp (name_j, "fr_FR.UTF-8") == 0); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } } } /* Check that gl_locale_name_thread returns a string that is allocated with indefinite extent. */ { /* Try many locale names in turn, in order to defeat possible caches. */ static const char * const choices[] = { "C", "POSIX", "af_ZA", "af_ZA.UTF-8", "am_ET", "am_ET.UTF-8", "be_BY", "be_BY.UTF-8", "bg_BG", "bg_BG.UTF-8", "ca_ES", "ca_ES.UTF-8", "cs_CZ", "cs_CZ.UTF-8", "da_DK", "da_DK.UTF-8", "de_AT", "de_AT.UTF-8", "de_CH", "de_CH.UTF-8", "de_DE", "de_DE.UTF-8", "el_GR", "el_GR.UTF-8", "en_AU", "en_AU.UTF-8", "en_CA", "en_CA.UTF-8", "en_GB", "en_GB.UTF-8", "en_IE", "en_IE.UTF-8", "en_NZ", "en_NZ.UTF-8", "en_US", "en_US.UTF-8", "es_ES", "es_ES.UTF-8", "et_EE", "et_EE.UTF-8", "eu_ES", "eu_ES.UTF-8", "fi_FI", "fi_FI.UTF-8", "fr_BE", "fr_BE.UTF-8", "fr_CA", "fr_CA.UTF-8", "fr_CH", "fr_CH.UTF-8", "fr_FR", "fr_FR.UTF-8", "he_IL", "he_IL.UTF-8", "hr_HR", "hr_HR.UTF-8", "hu_HU", "hu_HU.UTF-8", "hy_AM", "is_IS", "is_IS.UTF-8", "it_CH", "it_CH.UTF-8", "it_IT", "it_IT.UTF-8", "ja_JP.UTF-8", "kk_KZ", "kk_KZ.UTF-8", "ko_KR.UTF-8", "lt_LT", "lt_LT.UTF-8", "nl_BE", "nl_BE.UTF-8", "nl_NL", "nl_NL.UTF-8", "no_NO", "no_NO.UTF-8", "pl_PL", "pl_PL.UTF-8", "pt_BR", "pt_BR.UTF-8", "pt_PT", "pt_PT.UTF-8", "ro_RO", "ro_RO.UTF-8", "ru_RU", "ru_RU.UTF-8", "sk_SK", "sk_SK.UTF-8", "sl_SI", "sl_SI.UTF-8", "sv_SE", "sv_SE.UTF-8", "tr_TR", "tr_TR.UTF-8", "uk_UA", "uk_UA.UTF-8", "zh_CN", "zh_CN.UTF-8", "zh_HK", "zh_HK.UTF-8", "zh_TW", "zh_TW.UTF-8" }; /* Remember which locales are available. */ unsigned char /* bool */ available[SIZEOF (choices)]; /* Array of remembered results of gl_locale_name_thread. */ const char *unsaved_names[SIZEOF (choices)][SIZEOF (categories)]; /* Array of remembered results of gl_locale_name_thread, stored in safe memory. */ char *saved_names[SIZEOF (choices)][SIZEOF (categories)]; unsigned int j; for (j = 0; j < SIZEOF (choices); j++) { locale_t locale = newlocale (LC_ALL_MASK, choices[j], NULL); available[j] = (locale != NULL); if (locale != NULL) { unsigned int i; uselocale (locale); for (i = 0; i < SIZEOF (categories); i++) { unsaved_names[j][i] = gl_locale_name_thread (categories[i].cat, categories[i].string); saved_names[j][i] = strdup (unsaved_names[j][i]); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Verify the unsaved_names are still valid. */ for (j = 0; j < SIZEOF (choices); j++) if (available[j]) { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) ASSERT (strcmp (unsaved_names[j][i], saved_names[j][i]) == 0); } /* Allocate many locales, without freeing them. This is an attempt at overwriting as much of the previously allocated memory as possible. */ for (j = SIZEOF (choices); j > 0; ) { j--; if (available[j]) { locale_t locale = newlocale (LC_ALL_MASK, choices[j], NULL); unsigned int i; ASSERT (locale != NULL); uselocale (locale); for (i = 0; i < SIZEOF (categories); i++) { const char *name = gl_locale_name_thread (categories[i].cat, categories[i].string); ASSERT (strcmp (unsaved_names[j][i], name) == 0); } uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } /* Verify the unsaved_names are still valid. */ for (j = 0; j < SIZEOF (choices); j++) if (available[j]) { unsigned int i; for (i = 0; i < SIZEOF (categories); i++) { ASSERT (strcmp (unsaved_names[j][i], saved_names[j][i]) == 0); free (saved_names[j][i]); } } } #else /* Check that gl_locale_name_thread always returns NULL. */ ASSERT (gl_locale_name_thread (LC_CTYPE, "LC_CTYPE") == NULL); ASSERT (gl_locale_name_thread (LC_MESSAGES, "LC_MESSAGES") == NULL); #endif } /* Test the gl_locale_name_posix() function. */ static void test_locale_name_posix (void) { const char *name; /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE && HAVE_USELOCALE uselocale (LC_GLOBAL_LOCALE); #endif /* Check that when all environment variables are unset, gl_locale_name_posix returns either NULL or the default locale. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LC_NUMERIC"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); name = gl_locale_name_posix (LC_NUMERIC, "LC_NUMERIC"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); /* Check that an empty environment variable is treated like an unset environment variable. */ setenv ("LC_ALL", "", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "", 1); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "", 1); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); /* Check that LC_ALL overrides the others, and LANG is overridden by the others. */ setenv ("LC_ALL", "C", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "C", 1); setenv ("LC_MESSAGES", "C", 1); unsetenv ("LANG"); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); /* Check mixed situations. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); setenv ("LANG", "de_DE.UTF-8", 1); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name_posix (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "de_DE.UTF-8") == 0); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); unsetenv ("LANG"); if (setlocale (LC_ALL, "") != NULL) { name = gl_locale_name_posix (LC_CTYPE, "LC_CTYPE"); ASSERT (name == NULL || strcmp (name, gl_locale_name_default ()) == 0); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); } #if HAVE_NEWLOCALE && HAVE_USELOCALE /* Check that gl_locale_name_posix ignores the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); uselocale (locale); name = gl_locale_name_posix (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } #endif } /* Test the gl_locale_name_environ() function. */ static void test_locale_name_environ (void) { const char *name; /* Get into a defined state, */ setlocale (LC_ALL, "en_US.UTF-8"); #if HAVE_NEWLOCALE && HAVE_USELOCALE uselocale (LC_GLOBAL_LOCALE); #endif /* Check that when all environment variables are unset, gl_locale_name_environ returns NULL. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LC_NUMERIC"); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); ASSERT (gl_locale_name_environ (LC_NUMERIC, "LC_NUMERIC") == NULL); /* Check that an empty environment variable is treated like an unset environment variable. */ setenv ("LC_ALL", "", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "", 1); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "", 1); unsetenv ("LANG"); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "", 1); ASSERT (gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES") == NULL); /* Check that LC_ALL overrides the others, and LANG is overridden by the others. */ setenv ("LC_ALL", "C", 1); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); unsetenv ("LANG"); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); setenv ("LC_CTYPE", "C", 1); setenv ("LC_MESSAGES", "C", 1); unsetenv ("LANG"); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); /* Check mixed situations. */ unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); setenv ("LANG", "de_DE.UTF-8", 1); name = gl_locale_name_environ (LC_CTYPE, "LC_CTYPE"); ASSERT (strcmp (name, "de_DE.UTF-8") == 0); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); setenv ("LC_MESSAGES", "fr_FR.UTF-8", 1); unsetenv ("LANG"); name = gl_locale_name_environ (LC_CTYPE, "LC_CTYPE"); ASSERT (name == NULL); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "fr_FR.UTF-8") == 0); #if HAVE_NEWLOCALE && HAVE_USELOCALE /* Check that gl_locale_name_environ ignores the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { unsetenv ("LC_ALL"); unsetenv ("LC_CTYPE"); unsetenv ("LC_MESSAGES"); setenv ("LANG", "C", 1); setlocale (LC_ALL, ""); uselocale (locale); name = gl_locale_name_environ (LC_MESSAGES, "LC_MESSAGES"); ASSERT (strcmp (name, "C") == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } #endif } /* Test the gl_locale_name_default() function. */ static void test_locale_name_default (void) { const char *name = gl_locale_name_default (); ASSERT (name != NULL); /* Only Mac OS X and Windows have a facility for the user to set the default locale. */ #if !((defined __APPLE__ && defined __MACH__) || (defined _WIN32 || defined __WIN32__ || defined __CYGWIN__)) ASSERT (strcmp (name, "C") == 0); #endif #if HAVE_NEWLOCALE && HAVE_USELOCALE /* Check that gl_locale_name_default ignores the thread locale. */ { locale_t locale = newlocale (LC_ALL_MASK, "fr_FR.UTF-8", NULL); if (locale != NULL) { uselocale (locale); ASSERT (strcmp (gl_locale_name_default (), name) == 0); uselocale (LC_GLOBAL_LOCALE); freelocale (locale); } } #endif } int main () { test_locale_name (); test_locale_name_thread (); test_locale_name_posix (); test_locale_name_environ (); test_locale_name_default (); return 0; } gnuastro-0.5/bootstrapped/tests/test-localeconv.c0000644000175000017500000000442613217200024017254 00000000000000/* Test of localeconv() function. Copyright (C) 2012-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2012. */ #include #include #include "signature.h" SIGNATURE_CHECK (localeconv, struct lconv *, (void)); #include #include #include "macros.h" int main () { /* Test localeconv() result in the "C" locale. */ { struct lconv *l = localeconv (); ASSERT (STREQ (l->decimal_point, ".")); ASSERT (STREQ (l->thousands_sep, "")); #if !((defined __FreeBSD__ || defined __DragonFly__) || defined __sun) ASSERT (STREQ (l->grouping, "")); #endif ASSERT (STREQ (l->mon_decimal_point, "")); ASSERT (STREQ (l->mon_thousands_sep, "")); #if !((defined __FreeBSD__ || defined __DragonFly__) || defined __sun) ASSERT (STREQ (l->mon_grouping, "")); #endif ASSERT (STREQ (l->positive_sign, "")); ASSERT (STREQ (l->negative_sign, "")); ASSERT (STREQ (l->currency_symbol, "")); ASSERT (l->frac_digits == CHAR_MAX); ASSERT (l->p_cs_precedes == CHAR_MAX); ASSERT (l->p_sign_posn == CHAR_MAX); ASSERT (l->p_sep_by_space == CHAR_MAX); ASSERT (l->n_cs_precedes == CHAR_MAX); ASSERT (l->n_sign_posn == CHAR_MAX); ASSERT (l->n_sep_by_space == CHAR_MAX); ASSERT (STREQ (l->int_curr_symbol, "")); ASSERT (l->int_frac_digits == CHAR_MAX); ASSERT (l->int_p_cs_precedes == CHAR_MAX); ASSERT (l->int_p_sign_posn == CHAR_MAX); ASSERT (l->int_p_sep_by_space == CHAR_MAX); ASSERT (l->int_n_cs_precedes == CHAR_MAX); ASSERT (l->int_n_sign_posn == CHAR_MAX); ASSERT (l->int_n_sep_by_space == CHAR_MAX); } return 0; } gnuastro-0.5/bootstrapped/tests/test-locale.c0000644000175000017500000000441413217200024016363 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include "verify.h" int a[] = { LC_ALL, LC_COLLATE, LC_CTYPE, LC_MESSAGES, LC_MONETARY, LC_NUMERIC, LC_TIME }; /* Check that the 'struct lconv' type is defined. */ struct lconv l; int ls; /* Check that NULL can be passed through varargs as a pointer type, per POSIX 2008. */ verify (sizeof NULL == sizeof (void *)); int main () { #if HAVE_NEWLOCALE /* Check that the locale_t type and the LC_GLOBAL_LOCALE macro are defined. */ locale_t b = LC_GLOBAL_LOCALE; (void) b; #endif /* Check that 'struct lconv' has the ISO C and POSIX specified members. */ ls += sizeof (*l.decimal_point); ls += sizeof (*l.thousands_sep); ls += sizeof (*l.grouping); ls += sizeof (*l.mon_decimal_point); ls += sizeof (*l.mon_thousands_sep); ls += sizeof (*l.mon_grouping); ls += sizeof (*l.positive_sign); ls += sizeof (*l.negative_sign); ls += sizeof (*l.currency_symbol); ls += sizeof (l.frac_digits); ls += sizeof (l.p_cs_precedes); ls += sizeof (l.p_sign_posn); ls += sizeof (l.p_sep_by_space); ls += sizeof (l.n_cs_precedes); ls += sizeof (l.n_sign_posn); ls += sizeof (l.n_sep_by_space); ls += sizeof (*l.int_curr_symbol); ls += sizeof (l.int_frac_digits); ls += sizeof (l.int_p_cs_precedes); ls += sizeof (l.int_p_sign_posn); ls += sizeof (l.int_p_sep_by_space); ls += sizeof (l.int_n_cs_precedes); ls += sizeof (l.int_n_sign_posn); ls += sizeof (l.int_n_sep_by_space); return 0; } gnuastro-0.5/bootstrapped/tests/test-listen.c0000644000175000017500000000234213217200024016420 00000000000000/* Test listen() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (listen, int, (int, int)); #include #include #include "sockets.h" #include "macros.h" int main (void) { (void) gl_sockets_startup (SOCKETS_1_1); /* Test behaviour for invalid file descriptors. */ { errno = 0; ASSERT (listen (-1, 1) == -1); ASSERT (errno == EBADF); } { close (99); errno = 0; ASSERT (listen (99 ,1) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.5/bootstrapped/tests/test-limits-h.c0000644000175000017500000000311313217200024016645 00000000000000/* Test of substitute. Copyright 2016-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ #include #include #include "verify.h" #if 4 < __GNUC__ + (3 <= __GNUC_MINOR__) # pragma GCC diagnostic ignored "-Woverlength-strings" #endif /* Macros specified by ISO/IEC TS 18661-1:2014. */ #define verify_width(width, min, max) \ verify ((max) >> ((width) - 1 - ((min) < 0)) == 1) verify_width (CHAR_WIDTH, CHAR_MIN, CHAR_MAX); verify_width (SCHAR_WIDTH, SCHAR_MIN, SCHAR_MAX); verify_width (UCHAR_WIDTH, 0, UCHAR_MAX); verify_width (SHRT_WIDTH, SHRT_MIN, SHRT_MAX); verify_width (USHRT_WIDTH, 0, USHRT_MAX); verify_width (INT_WIDTH, INT_MIN, INT_MAX); verify_width (UINT_WIDTH, 0, UINT_MAX); verify_width (LONG_WIDTH, LONG_MIN, LONG_MAX); verify_width (ULONG_WIDTH, 0, ULONG_MAX); verify_width (LLONG_WIDTH, LLONG_MIN, LLONG_MAX); verify_width (ULLONG_WIDTH, 0, ULLONG_MAX); int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-langinfo.c0000644000175000017500000000357213217200024016725 00000000000000/* Test of substitute. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include #include /* Check that all the nl_item values are defined. */ int items[] = { /* nl_langinfo items of the LC_CTYPE category */ CODESET, /* nl_langinfo items of the LC_NUMERIC category */ RADIXCHAR, THOUSEP, /* nl_langinfo items of the LC_TIME category */ D_T_FMT, D_FMT, T_FMT, T_FMT_AMPM, AM_STR, PM_STR, DAY_1, DAY_2, DAY_3, DAY_4, DAY_5, DAY_6, DAY_7, ABDAY_1, ABDAY_2, ABDAY_3, ABDAY_4, ABDAY_5, ABDAY_6, ABDAY_7, MON_1, MON_2, MON_3, MON_4, MON_5, MON_6, MON_7, MON_8, MON_9, MON_10, MON_11, MON_12, ABMON_1, ABMON_2, ABMON_3, ABMON_4, ABMON_5, ABMON_6, ABMON_7, ABMON_8, ABMON_9, ABMON_10, ABMON_11, ABMON_12, ERA, ERA_D_FMT, ERA_D_T_FMT, ERA_T_FMT, ALT_DIGITS, /* nl_langinfo items of the LC_MONETARY category */ CRNCYSTR, /* nl_langinfo items of the LC_MESSAGES category */ YESEXPR, NOEXPR }; int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-iswblank.c0000644000175000017500000000204313217200024016732 00000000000000/* Test of iswblank() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "macros.h" /* Check that WEOF is defined. */ wint_t e = WEOF; int main (void) { /* Check that the function exist as a function or as a macro. */ (void) iswblank (0); /* Check that the isw* functions map WEOF to 0. */ ASSERT (!iswblank (e)); return 0; } gnuastro-0.5/bootstrapped/tests/test-isnanl-nolibm.c0000644000175000017500000000155413217200024017670 00000000000000/* Test of isnanl() substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "isnanl-nolibm.h" #include "test-isnanl.h" gnuastro-0.5/bootstrapped/tests/test-isnanf-nolibm.c0000644000175000017500000000145513217200024017662 00000000000000/* Test of isnanf() substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "isnanf-nolibm.h" #include "test-isnanf.h" gnuastro-0.5/bootstrapped/tests/test-isnand-nolibm.c0000644000175000017500000000145513217200024017660 00000000000000/* Test of isnand() substitute. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "isnand-nolibm.h" #include "test-isnand.h" gnuastro-0.5/bootstrapped/tests/test-isblank.c0000644000175000017500000000305013217200024016542 00000000000000/* Test of isblank() function. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (isblank, int, (int)); #include #include #include "macros.h" int main (int argc, char *argv[]) { unsigned int c; /* Verify the property in the "C" locale. POSIX specifies in that - in all locales, the blank characters include the and characters, - in the "POSIX" locale (which is usually the same as the "C" locale), the blank characters include only the ASCII and characters. */ for (c = 0; c <= UCHAR_MAX; c++) ASSERT (!isblank (c) == !(c == ' ' || c == '\t')); ASSERT (!isblank (EOF)); return 0; } gnuastro-0.5/bootstrapped/tests/test-ioctl.c0000644000175000017500000000241513217200023016234 00000000000000/* Test of ioctl() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "signature.h" SIGNATURE_CHECK (ioctl, int, (int, int, ...)); #include #include #include "macros.h" int main (void) { #ifdef FIONREAD /* Test behaviour for invalid file descriptors. */ { int value; errno = 0; ASSERT (ioctl (-1, FIONREAD, &value) == -1); ASSERT (errno == EBADF); } { int value; close (99); errno = 0; ASSERT (ioctl (99, FIONREAD, &value) == -1); ASSERT (errno == EBADF); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-inttypes.c0000644000175000017500000000606113217200023017002 00000000000000/* Test of substitute. Copyright (C) 2006-2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #include /* Tests for macros supposed to be defined in inttypes.h. */ const char *k = /* implicit string concatenation */ #ifdef INT8_MAX PRId8 PRIi8 #endif #ifdef UINT8_MAX PRIo8 PRIu8 PRIx8 PRIX8 #endif #ifdef INT16_MAX PRId16 PRIi16 #endif #ifdef UINT16_MAX PRIo16 PRIu16 PRIx16 PRIX16 #endif #ifdef INT32_MAX PRId32 PRIi32 #endif #ifdef UINT32_MAX PRIo32 PRIu32 PRIx32 PRIX32 #endif #ifdef INT64_MAX PRId64 PRIi64 #endif #ifdef UINT64_MAX PRIo64 PRIu64 PRIx64 PRIX64 #endif PRIdLEAST8 PRIiLEAST8 PRIoLEAST8 PRIuLEAST8 PRIxLEAST8 PRIXLEAST8 PRIdLEAST16 PRIiLEAST16 PRIoLEAST16 PRIuLEAST16 PRIxLEAST16 PRIXLEAST16 PRIdLEAST32 PRIiLEAST32 PRIoLEAST32 PRIuLEAST32 PRIxLEAST32 PRIXLEAST32 PRIdLEAST64 PRIiLEAST64 PRIoLEAST64 PRIuLEAST64 PRIxLEAST64 PRIXLEAST64 PRIdFAST8 PRIiFAST8 PRIoFAST8 PRIuFAST8 PRIxFAST8 PRIXFAST8 PRIdFAST16 PRIiFAST16 PRIoFAST16 PRIuFAST16 PRIxFAST16 PRIXFAST16 PRIdFAST32 PRIiFAST32 PRIoFAST32 PRIuFAST32 PRIxFAST32 PRIXFAST32 PRIdFAST64 PRIiFAST64 PRIoFAST64 PRIuFAST64 PRIxFAST64 PRIXFAST64 PRIdMAX PRIiMAX PRIoMAX PRIuMAX PRIxMAX PRIXMAX #ifdef INTPTR_MAX PRIdPTR PRIiPTR #endif #ifdef UINTPTR_MAX PRIoPTR PRIuPTR PRIxPTR PRIXPTR #endif ; const char *l = /* implicit string concatenation */ #ifdef INT8_MAX SCNd8 SCNi8 #endif #ifdef UINT8_MAX SCNo8 SCNu8 SCNx8 #endif #ifdef INT16_MAX SCNd16 SCNi16 #endif #ifdef UINT16_MAX SCNo16 SCNu16 SCNx16 #endif #ifdef INT32_MAX SCNd32 SCNi32 #endif #ifdef UINT32_MAX SCNo32 SCNu32 SCNx32 #endif #ifdef INT64_MAX SCNd64 SCNi64 #endif #ifdef UINT64_MAX SCNo64 SCNu64 SCNx64 #endif SCNdLEAST8 SCNiLEAST8 SCNoLEAST8 SCNuLEAST8 SCNxLEAST8 SCNdLEAST16 SCNiLEAST16 SCNoLEAST16 SCNuLEAST16 SCNxLEAST16 SCNdLEAST32 SCNiLEAST32 SCNoLEAST32 SCNuLEAST32 SCNxLEAST32 SCNdLEAST64 SCNiLEAST64 SCNoLEAST64 SCNuLEAST64 SCNxLEAST64 SCNdFAST8 SCNiFAST8 SCNoFAST8 SCNuFAST8 SCNxFAST8 SCNdFAST16 SCNiFAST16 SCNoFAST16 SCNuFAST16 SCNxFAST16 SCNdFAST32 SCNiFAST32 SCNoFAST32 SCNuFAST32 SCNxFAST32 SCNdFAST64 SCNiFAST64 SCNoFAST64 SCNuFAST64 SCNxFAST64 SCNdMAX SCNiMAX SCNoMAX SCNuMAX SCNxMAX #ifdef INTPTR_MAX SCNdPTR SCNiPTR #endif #ifdef UINTPTR_MAX SCNoPTR SCNuPTR SCNxPTR #endif ; int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-intprops.c0000644000175000017500000004343313217200023017005 00000000000000/* Test intprops.h. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ /* Tell gcc not to warn about the long expressions that the overflow macros expand to, or about the (X < 0) expressions. */ #if 4 < __GNUC__ + (3 <= __GNUC_MINOR__) # pragma GCC diagnostic ignored "-Woverlength-strings" # pragma GCC diagnostic ignored "-Wtype-limits" /* Work around a bug in GCC 6.1 and earlier; see: https://gcc.gnu.org/bugzilla/show_bug.cgi?id=68971 */ # pragma GCC diagnostic ignored "-Woverflow" #endif #include #include "intprops.h" #include "verify.h" #include #include #include #include "macros.h" /* VERIFY (X) uses a static assertion for compilers that are known to work, and falls back on a dynamic assertion for other compilers. These tests should be checkable via 'verify' rather than 'ASSERT', but using 'verify' would run into a bug with HP-UX 11.23 cc; see . */ #if __GNUC__ || __SUNPRO_C # define VERIFY(x) do { verify (x); } while (0) #else # define VERIFY(x) ASSERT (x) #endif #define DONTCARE __LINE__ int main (void) { /* Use VERIFY for tests that must be integer constant expressions, ASSERT otherwise. */ /* TYPE_IS_INTEGER. */ ASSERT (TYPE_IS_INTEGER (bool)); ASSERT (TYPE_IS_INTEGER (char)); ASSERT (TYPE_IS_INTEGER (signed char)); ASSERT (TYPE_IS_INTEGER (unsigned char)); ASSERT (TYPE_IS_INTEGER (short int)); ASSERT (TYPE_IS_INTEGER (unsigned short int)); ASSERT (TYPE_IS_INTEGER (int)); ASSERT (TYPE_IS_INTEGER (unsigned int)); ASSERT (TYPE_IS_INTEGER (long int)); ASSERT (TYPE_IS_INTEGER (unsigned long int)); ASSERT (TYPE_IS_INTEGER (intmax_t)); ASSERT (TYPE_IS_INTEGER (uintmax_t)); ASSERT (! TYPE_IS_INTEGER (float)); ASSERT (! TYPE_IS_INTEGER (double)); ASSERT (! TYPE_IS_INTEGER (long double)); /* TYPE_SIGNED. */ /* VERIFY (! TYPE_SIGNED (bool)); // not guaranteed by gnulib substitute */ VERIFY (TYPE_SIGNED (signed char)); VERIFY (! TYPE_SIGNED (unsigned char)); VERIFY (TYPE_SIGNED (short int)); VERIFY (! TYPE_SIGNED (unsigned short int)); VERIFY (TYPE_SIGNED (int)); VERIFY (! TYPE_SIGNED (unsigned int)); VERIFY (TYPE_SIGNED (long int)); VERIFY (! TYPE_SIGNED (unsigned long int)); VERIFY (TYPE_SIGNED (intmax_t)); VERIFY (! TYPE_SIGNED (uintmax_t)); ASSERT (TYPE_SIGNED (float)); ASSERT (TYPE_SIGNED (double)); ASSERT (TYPE_SIGNED (long double)); /* Integer representation. Check that it is two's complement. */ VERIFY (INT_MIN + INT_MAX < 0); /* TYPE_MINIMUM, TYPE_MAXIMUM. */ VERIFY (TYPE_MINIMUM (char) == CHAR_MIN); VERIFY (TYPE_MAXIMUM (char) == CHAR_MAX); VERIFY (TYPE_MINIMUM (unsigned char) == 0); VERIFY (TYPE_MAXIMUM (unsigned char) == UCHAR_MAX); VERIFY (TYPE_MINIMUM (signed char) == SCHAR_MIN); VERIFY (TYPE_MAXIMUM (signed char) == SCHAR_MAX); VERIFY (TYPE_MINIMUM (short int) == SHRT_MIN); VERIFY (TYPE_MAXIMUM (short int) == SHRT_MAX); VERIFY (TYPE_MINIMUM (unsigned short int) == 0); VERIFY (TYPE_MAXIMUM (unsigned short int) == USHRT_MAX); VERIFY (TYPE_MINIMUM (int) == INT_MIN); VERIFY (TYPE_MAXIMUM (int) == INT_MAX); VERIFY (TYPE_MINIMUM (unsigned int) == 0); VERIFY (TYPE_MAXIMUM (unsigned int) == UINT_MAX); VERIFY (TYPE_MINIMUM (long int) == LONG_MIN); VERIFY (TYPE_MAXIMUM (long int) == LONG_MAX); VERIFY (TYPE_MINIMUM (unsigned long int) == 0); VERIFY (TYPE_MAXIMUM (unsigned long int) == ULONG_MAX); #ifdef LLONG_MAX verify (TYPE_MINIMUM (long long int) == LLONG_MIN); verify (TYPE_MAXIMUM (long long int) == LLONG_MAX); #endif VERIFY (TYPE_MINIMUM (intmax_t) == INTMAX_MIN); VERIFY (TYPE_MAXIMUM (intmax_t) == INTMAX_MAX); VERIFY (TYPE_MINIMUM (uintmax_t) == 0); VERIFY (TYPE_MAXIMUM (uintmax_t) == UINTMAX_MAX); /* TYPE_WIDTH. */ #ifdef CHAR_WIDTH verify (TYPE_WIDTH (char) == CHAR_WIDTH); verify (TYPE_WIDTH (signed char) == SCHAR_WIDTH); verify (TYPE_WIDTH (unsigned char) == UCHAR_WIDTH); verify (TYPE_WIDTH (short int) == SHRT_WIDTH); verify (TYPE_WIDTH (unsigned short int) == USHRT_WIDTH); verify (TYPE_WIDTH (int) == INT_WIDTH); verify (TYPE_WIDTH (unsigned int) == UINT_WIDTH); verify (TYPE_WIDTH (long int) == LONG_WIDTH); verify (TYPE_WIDTH (unsigned long int) == ULONG_WIDTH); #ifdef LLONG_WIDTH verify (TYPE_WIDTH (long long int) == LLONG_WIDTH); verify (TYPE_WIDTH (unsigned long long int) == ULLONG_WIDTH); #endif #endif /* INT_BITS_STRLEN_BOUND. */ VERIFY (INT_BITS_STRLEN_BOUND (1) == 1); VERIFY (INT_BITS_STRLEN_BOUND (2620) == 789); /* INT_STRLEN_BOUND, INT_BUFSIZE_BOUND. */ #ifdef INT32_MAX /* POSIX guarantees int32_t; this ports to non-POSIX. */ VERIFY (INT_STRLEN_BOUND (int32_t) == sizeof ("-2147483648") - 1); VERIFY (INT_BUFSIZE_BOUND (int32_t) == sizeof ("-2147483648")); #endif #ifdef INT64_MAX VERIFY (INT_STRLEN_BOUND (int64_t) == sizeof ("-9223372036854775808") - 1); VERIFY (INT_BUFSIZE_BOUND (int64_t) == sizeof ("-9223372036854775808")); #endif /* All the INT__RANGE_OVERFLOW tests are equally valid as INT__OVERFLOW tests, so define macros to do both. OP is the operation, OPNAME its symbolic name, A and B its operands, T the result type, V the overflow flag, and VRES the result if V and if two's complement. CHECK_BINOP is for most binary operatinos, CHECK_SBINOP for binary +, -, * when the result type is signed, and CHECK_UNOP for unary operations. */ #define CHECK_BINOP(op, opname, a, b, t, v, vres) \ VERIFY (INT_##opname##_RANGE_OVERFLOW (a, b, TYPE_MINIMUM (t), \ TYPE_MAXIMUM (t)) \ == (v)); \ VERIFY (INT_##opname##_OVERFLOW (a, b) == (v)) #define CHECK_SBINOP(op, opname, a, b, t, v, vres) \ CHECK_BINOP(op, opname, a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_##opname##_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) op (b)))); \ } #define CHECK_UNOP(op, opname, a, t, v) \ VERIFY (INT_##opname##_RANGE_OVERFLOW (a, TYPE_MINIMUM (t), \ TYPE_MAXIMUM (t)) \ == (v)); \ VERIFY (INT_##opname##_OVERFLOW (a) == (v)) /* INT__RANGE_OVERFLOW, INT__OVERFLOW. */ VERIFY (INT_ADD_RANGE_OVERFLOW (INT_MAX, 1, INT_MIN, INT_MAX)); VERIFY (INT_ADD_OVERFLOW (INT_MAX, 1)); CHECK_SBINOP (+, ADD, INT_MAX, 1, int, true, INT_MIN); CHECK_SBINOP (+, ADD, INT_MAX, -1, int, false, INT_MAX - 1); CHECK_SBINOP (+, ADD, INT_MIN, 1, int, false, INT_MIN + 1); CHECK_SBINOP (+, ADD, INT_MIN, -1, int, true, INT_MAX); CHECK_BINOP (+, ADD, UINT_MAX, 1u, unsigned int, true, 0u); CHECK_BINOP (+, ADD, 0u, 1u, unsigned int, false, 1u); CHECK_SBINOP (-, SUBTRACT, INT_MAX, 1, int, false, INT_MAX - 1); CHECK_SBINOP (-, SUBTRACT, INT_MAX, -1, int, true, INT_MIN); CHECK_SBINOP (-, SUBTRACT, INT_MIN, 1, int, true, INT_MAX); CHECK_SBINOP (-, SUBTRACT, INT_MIN, -1, int, false, INT_MIN - -1); CHECK_BINOP (-, SUBTRACT, UINT_MAX, 1u, unsigned int, false, UINT_MAX - 1u); CHECK_BINOP (-, SUBTRACT, 0u, 1u, unsigned int, true, 0u - 1u); CHECK_UNOP (-, NEGATE, INT_MIN, int, true); CHECK_UNOP (-, NEGATE, 0, int, false); CHECK_UNOP (-, NEGATE, INT_MAX, int, false); CHECK_UNOP (-, NEGATE, 0u, unsigned int, false); CHECK_UNOP (-, NEGATE, 1u, unsigned int, true); CHECK_UNOP (-, NEGATE, UINT_MAX, unsigned int, true); CHECK_SBINOP (*, MULTIPLY, INT_MAX, INT_MAX, int, true, 1); CHECK_SBINOP (*, MULTIPLY, INT_MAX, INT_MIN, int, true, INT_MIN); CHECK_SBINOP (*, MULTIPLY, INT_MIN, INT_MAX, int, true, INT_MIN); CHECK_SBINOP (*, MULTIPLY, INT_MIN, INT_MIN, int, true, 0); CHECK_SBINOP (*, MULTIPLY, -1, INT_MIN, int, INT_NEGATE_OVERFLOW (INT_MIN), INT_MIN); CHECK_SBINOP (*, MULTIPLY, LONG_MIN / INT_MAX, (long int) INT_MAX, long int, false, LONG_MIN - LONG_MIN % INT_MAX); CHECK_BINOP (/, DIVIDE, INT_MIN, -1, int, INT_NEGATE_OVERFLOW (INT_MIN), INT_MIN); CHECK_BINOP (/, DIVIDE, INT_MAX, 1, int, false, INT_MAX); CHECK_BINOP (/, DIVIDE, (unsigned int) INT_MIN, -1u, unsigned int, false, INT_MIN / -1u); CHECK_BINOP (%, REMAINDER, INT_MIN, -1, int, INT_NEGATE_OVERFLOW (INT_MIN), 0); CHECK_BINOP (%, REMAINDER, INT_MAX, 1, int, false, 0); CHECK_BINOP (%, REMAINDER, (unsigned int) INT_MIN, -1u, unsigned int, false, INT_MIN % -1u); CHECK_BINOP (<<, LEFT_SHIFT, UINT_MAX, 1, unsigned int, true, UINT_MAX << 1); CHECK_BINOP (<<, LEFT_SHIFT, UINT_MAX / 2 + 1, 1, unsigned int, true, (UINT_MAX / 2 + 1) << 1); CHECK_BINOP (<<, LEFT_SHIFT, UINT_MAX / 2, 1, unsigned int, false, (UINT_MAX / 2) << 1); /* INT__OVERFLOW and INT__WRAPV with mixed types. */ #define CHECK_SUM(a, b, t, v, vres) \ CHECK_SUM1(a, b, t, v, vres); \ CHECK_SUM1(b, a, t, v, vres) #define CHECK_SSUM(a, b, t, v, vres) \ CHECK_SSUM1(a, b, t, v, vres); \ CHECK_SSUM1(b, a, t, v, vres) #define CHECK_SUM1(a, b, t, v, vres) \ VERIFY (INT_ADD_OVERFLOW (a, b) == (v)) #define CHECK_SSUM1(a, b, t, v, vres) \ CHECK_SUM1(a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_ADD_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) + (b)))); \ } CHECK_SSUM (-1, LONG_MIN, long int, true, LONG_MAX); CHECK_SUM (-1, UINT_MAX, unsigned int, false, DONTCARE); CHECK_SSUM (-1L, INT_MIN, long int, INT_MIN == LONG_MIN, INT_MIN == LONG_MIN ? INT_MAX : DONTCARE); CHECK_SUM (0u, -1, unsigned int, true, 0u + -1); CHECK_SUM (0u, 0, unsigned int, false, DONTCARE); CHECK_SUM (0u, 1, unsigned int, false, DONTCARE); CHECK_SSUM (1, LONG_MAX, long int, true, LONG_MIN); CHECK_SUM (1, UINT_MAX, unsigned int, true, 0u); CHECK_SSUM (1L, INT_MAX, long int, INT_MAX == LONG_MAX, INT_MAX == LONG_MAX ? INT_MIN : DONTCARE); CHECK_SUM (1u, INT_MAX, unsigned int, INT_MAX == UINT_MAX, 1u + INT_MAX); CHECK_SUM (1u, INT_MIN, unsigned int, true, 1u + INT_MIN); { long int result; ASSERT (INT_ADD_WRAPV (1, INT_MAX, &result) == (INT_MAX == LONG_MAX)); ASSERT (INT_ADD_WRAPV (-1, INT_MIN, &result) == (INT_MIN == LONG_MIN)); } #define CHECK_DIFFERENCE(a, b, t, v, vres) \ VERIFY (INT_SUBTRACT_OVERFLOW (a, b) == (v)) #define CHECK_SDIFFERENCE(a, b, t, v, vres) \ CHECK_DIFFERENCE(a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_SUBTRACT_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) - (b)))); \ } CHECK_DIFFERENCE (INT_MAX, 1u, unsigned int, UINT_MAX < INT_MAX - 1, INT_MAX - 1u); CHECK_DIFFERENCE (UINT_MAX, 1, unsigned int, false, UINT_MAX - 1); CHECK_DIFFERENCE (0u, -1, unsigned int, false, 0u - -1); CHECK_DIFFERENCE (UINT_MAX, -1, unsigned int, true, UINT_MAX - -1); CHECK_DIFFERENCE (INT_MIN, 1u, unsigned int, true, INT_MIN - 1u); CHECK_DIFFERENCE (-1, 0u, unsigned int, true, -1 - 0u); CHECK_SDIFFERENCE (-1, INT_MIN, int, false, -1 - INT_MIN); CHECK_SDIFFERENCE (-1, INT_MAX, int, false, -1 - INT_MAX); CHECK_SDIFFERENCE (0, INT_MIN, int, INT_MIN < -INT_MAX, INT_MIN); CHECK_SDIFFERENCE (0, INT_MAX, int, false, 0 - INT_MAX); { long int result; ASSERT (INT_SUBTRACT_WRAPV (INT_MAX, -1, &result) == (INT_MAX == LONG_MAX)); ASSERT (INT_SUBTRACT_WRAPV (INT_MIN, 1, &result) == (INT_MAX == LONG_MAX)); } #define CHECK_PRODUCT(a, b, t, v, vres) \ CHECK_PRODUCT1(a, b, t, v, vres); \ CHECK_PRODUCT1(b, a, t, v, vres) #define CHECK_SPRODUCT(a, b, t, v, vres) \ CHECK_SPRODUCT1(a, b, t, v, vres); \ CHECK_SPRODUCT1(b, a, t, v, vres) #define CHECK_PRODUCT1(a, b, t, v, vres) \ VERIFY (INT_MULTIPLY_OVERFLOW (a, b) == (v)) #define CHECK_SPRODUCT1(a, b, t, v, vres) \ CHECK_PRODUCT1(a, b, t, v, vres); \ { \ t result; \ ASSERT (INT_MULTIPLY_WRAPV (a, b, &result) == (v)); \ ASSERT (result == ((v) ? (vres) : ((a) * (b)))); \ } CHECK_PRODUCT (-1, 1u, unsigned int, true, -1 * 1u); CHECK_SPRODUCT (-1, INT_MIN, int, INT_NEGATE_OVERFLOW (INT_MIN), INT_MIN); CHECK_PRODUCT (-1, UINT_MAX, unsigned int, true, -1 * UINT_MAX); CHECK_SPRODUCT (-32768, LONG_MAX / -32768 - 1, long int, true, LONG_MIN); CHECK_SPRODUCT (-12345, LONG_MAX / -12345, long int, false, DONTCARE); CHECK_SPRODUCT (0, -1, int, false, DONTCARE); CHECK_SPRODUCT (0, 0, int, false, DONTCARE); CHECK_PRODUCT (0, 0u, unsigned int, false, DONTCARE); CHECK_SPRODUCT (0, 1, int, false, DONTCARE); CHECK_SPRODUCT (0, INT_MAX, int, false, DONTCARE); CHECK_SPRODUCT (0, INT_MIN, int, false, DONTCARE); CHECK_PRODUCT (0, UINT_MAX, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, -1, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, 0, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, 0u, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, 1, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, INT_MAX, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, INT_MIN, unsigned int, false, DONTCARE); CHECK_PRODUCT (0u, UINT_MAX, unsigned int, false, DONTCARE); CHECK_SPRODUCT (1, INT_MAX, int, false, DONTCARE); CHECK_SPRODUCT (1, INT_MIN, int, false, DONTCARE); CHECK_PRODUCT (1, UINT_MAX, unsigned int, false, DONTCARE); CHECK_PRODUCT (1u, INT_MIN, unsigned int, true, 1u * INT_MIN); CHECK_PRODUCT (1u, INT_MAX, unsigned int, UINT_MAX < INT_MAX, 1u * INT_MAX); CHECK_PRODUCT (INT_MAX, UINT_MAX, unsigned int, true, INT_MAX * UINT_MAX); CHECK_PRODUCT (INT_MAX, ULONG_MAX, unsigned long int, true, INT_MAX * ULONG_MAX); CHECK_SPRODUCT (INT_MIN, LONG_MAX / INT_MIN - 1, long int, true, LONG_MIN); CHECK_SPRODUCT (INT_MIN, LONG_MAX / INT_MIN, long int, false, DONTCARE); CHECK_PRODUCT (INT_MIN, UINT_MAX, unsigned int, true, INT_MIN * UINT_MAX); CHECK_PRODUCT (INT_MIN, ULONG_MAX, unsigned long int, true, INT_MIN * ULONG_MAX); { long int result; ASSERT (INT_MULTIPLY_WRAPV (INT_MAX, INT_MAX, &result) == (LONG_MAX / INT_MAX < INT_MAX)); ASSERT (INT_MULTIPLY_WRAPV (INT_MAX, INT_MAX, &result) || result == INT_MAX * (long int) INT_MAX); ASSERT (INT_MULTIPLY_WRAPV (INT_MIN, INT_MIN, &result) || result == INT_MIN * (long int) INT_MIN); } # ifdef LLONG_MAX { long long int result; ASSERT (INT_MULTIPLY_WRAPV (LONG_MAX, LONG_MAX, &result) == (LLONG_MAX / LONG_MAX < LONG_MAX)); ASSERT (INT_MULTIPLY_WRAPV (LONG_MAX, LONG_MAX, &result) || result == LONG_MAX * (long long int) LONG_MAX); ASSERT (INT_MULTIPLY_WRAPV (LONG_MIN, LONG_MIN, &result) || result == LONG_MIN * (long long int) LONG_MIN); } # endif #define CHECK_QUOTIENT(a, b, v) VERIFY (INT_DIVIDE_OVERFLOW (a, b) == (v)) CHECK_QUOTIENT (INT_MIN, -1L, INT_MIN == LONG_MIN); CHECK_QUOTIENT (INT_MIN, UINT_MAX, false); CHECK_QUOTIENT (INTMAX_MIN, UINTMAX_MAX, false); CHECK_QUOTIENT (INTMAX_MIN, UINT_MAX, false); CHECK_QUOTIENT (-11, 10u, true); CHECK_QUOTIENT (-10, 10u, true); CHECK_QUOTIENT (-9, 10u, false); CHECK_QUOTIENT (11u, -10, true); CHECK_QUOTIENT (10u, -10, true); CHECK_QUOTIENT (9u, -10, false); #define CHECK_REMAINDER(a, b, v) VERIFY (INT_REMAINDER_OVERFLOW (a, b) == (v)) CHECK_REMAINDER (INT_MIN, -1L, INT_MIN == LONG_MIN); CHECK_REMAINDER (-1, UINT_MAX, true); CHECK_REMAINDER ((intmax_t) -1, UINTMAX_MAX, true); CHECK_REMAINDER (INTMAX_MIN, UINT_MAX, (INTMAX_MAX < UINT_MAX && - (unsigned int) INTMAX_MIN % UINT_MAX != 0)); CHECK_REMAINDER (INT_MIN, ULONG_MAX, INT_MIN % ULONG_MAX != 1); CHECK_REMAINDER (1u, -1, false); CHECK_REMAINDER (37*39u, -39, false); CHECK_REMAINDER (37*39u + 1, -39, true); CHECK_REMAINDER (37*39u - 1, -39, true); CHECK_REMAINDER (LONG_MAX, -INT_MAX, false); return 0; } gnuastro-0.5/bootstrapped/tests/test-inet_pton.c0000644000175000017500000000333013217200023017116 00000000000000/* Test of inet_pton function. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (inet_pton, int, (int, const char *, void *)); #include #include #include "macros.h" int main (void) { #if defined AF_INET /* HAVE_IPV4 */ { /* This machine was for a long time known as ma2s2.mathematik.uni-karlsruhe.de. */ const char printable[] = "129.13.115.2"; struct in_addr internal; int ret; ret = inet_pton (AF_INET, printable, &internal); ASSERT (ret == 1); /* Verify that internal is filled in network byte order. */ ASSERT (((unsigned char *) &internal)[0] == 0x81); ASSERT (((unsigned char *) &internal)[1] == 0x0D); ASSERT (((unsigned char *) &internal)[2] == 0x73); ASSERT (((unsigned char *) &internal)[3] == 0x02); # ifdef WORDS_BIGENDIAN ASSERT (internal.s_addr == 0x810D7302); # else ASSERT (internal.s_addr == 0x02730D81); # endif } #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-ignore-value.c0000644000175000017500000000365213217200023017523 00000000000000/* Test the "ignore-value" module. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake. */ #include #include "ignore-value.h" #include #ifndef _GL_ATTRIBUTE_RETURN_CHECK # if __GNUC__ < 3 || (__GNUC__ == 3 && __GNUC_MINOR__ < 4) # define _GL_ATTRIBUTE_RETURN_CHECK # else # define _GL_ATTRIBUTE_RETURN_CHECK __attribute__((__warn_unused_result__)) # endif #endif struct s { int i; }; static char doChar (void) _GL_ATTRIBUTE_RETURN_CHECK; static int doInt (void) _GL_ATTRIBUTE_RETURN_CHECK; static off_t doOff (void) _GL_ATTRIBUTE_RETURN_CHECK; static void *doPtr (void) _GL_ATTRIBUTE_RETURN_CHECK; static struct s doStruct (void) _GL_ATTRIBUTE_RETURN_CHECK; static char doChar (void) { return 0; } static int doInt (void) { return 0; } static off_t doOff (void) { return 0; } static void * doPtr (void) { return NULL; } static struct s doStruct (void) { static struct s s1; return s1; } int main (void) { /* If this test can compile with -Werror and the same warnings as the rest of the project, then we are properly silencing warnings about ignored return values. */ ignore_value (doChar ()); ignore_value (doInt ()); ignore_value (doOff ()); ignore_value (doPtr ()); ignore_value (doStruct ()); return 0; } gnuastro-0.5/bootstrapped/tests/test-gettimeofday.c0000644000175000017500000000245113217200023017603 00000000000000/* * Copyright (C) 2005, 2007, 2009-2017 Free Software Foundation, Inc. * Written by Jim Meyering. * * This program is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation; either version 3 of the License, or * (at your option) any later version. * * This program is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (gettimeofday, int, (struct timeval *, GETTIMEOFDAY_TIMEZONE *)); #include #include #include int main (void) { time_t t = 0; struct tm *lt; struct tm saved_lt; struct timeval tv; lt = localtime (&t); saved_lt = *lt; gettimeofday (&tv, NULL); if (memcmp (lt, &saved_lt, sizeof (struct tm)) != 0) { fprintf (stderr, "gettimeofday still clobbers the localtime buffer!\n"); return 1; } return 0; } gnuastro-0.5/bootstrapped/tests/test-getprogname.c0000644000175000017500000000400713217200023017431 00000000000000/* Test the gnulib getprogname module. Copyright (C) 2016-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "getprogname.h" #include #include #ifdef __hpux # define STREQ(a, b) (strncmp (a, b, 14) == 0) #else # define STREQ(a, b) (strcmp (a, b) == 0) #endif int main (void) { char const *p = getprogname (); /* libtool creates a temporary executable whose name is sometimes prefixed with "lt-" (depends on the platform). But the name of the temporary executable is a detail that should not be visible to the end user and to the test suite. Remove this "lt-" prefix here. */ if (strncmp (p, "lt-", 3) == 0) p += 3; /* Note: You can make this test fail a) by running it on a case-insensitive file system (such as on Windows, Cygwin, or on Mac OS X with a case-insensitive HFS+ file system), with an invocation that contains upper case characters, e.g. test-GETPROGNAME, b) by hardlinking or symlinking it to a different name (e.g. test-foo) and invoking it through that name. That's not the intended use. The Makefile always invokes it as 'test-getprogname${EXEEXT}'. */ #if defined __CYGWIN__ /* The Cygwin getprogname() function strips the ".exe" suffix. */ assert (STREQ (p, "test-getprogname")); #else assert (STREQ (p, "test-getprogname" EXEEXT)); #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-getopt-posix.c0000644000175000017500000000273213217200023017566 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* None of the files accessed by this test are large, so disable the ftell link warning if we are not using the gnulib ftell module. */ #define _GL_NO_LARGE_FILES /* POSIX and glibc provide the getopt() function in , see http://pubs.opengroup.org/onlinepubs/9699919799/functions/getopt.html https://www.gnu.org/software/libc/manual/html_node/Using-Getopt.html But gnulib provides the getopt() function in , not in . Nevertheless the getopt() function should also be found in . */ #include #define TEST_GETOPT_GNU 0 #define TEST_GETOPT_TMP_NAME "test-getopt-posix.tmp" #include "test-getopt-main.h" gnuastro-0.5/bootstrapped/tests/test-getopt-gnu.c0000644000175000017500000000363013217200023017213 00000000000000/* Test of command line argument processing. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* None of the files accessed by this test are large, so disable the ftell link warning if we are not using the gnulib ftell module. */ #define _GL_NO_LARGE_FILES /* POSIX and glibc provide the getopt() function in , see http://pubs.opengroup.org/onlinepubs/9699919799/functions/getopt.html https://www.gnu.org/software/libc/manual/html_node/Using-Getopt.html But gnulib provides the getopt() function in , not in . This is what we are testing here. */ #include #ifndef __getopt_argv_const # define __getopt_argv_const const #endif #include "signature.h" SIGNATURE_CHECK (getopt_long, int, (int, char *__getopt_argv_const *, char const *, struct option const *, int *)); SIGNATURE_CHECK (getopt_long_only, int, (int, char *__getopt_argv_const *, char const *, struct option const *, int *)); #define TEST_GETOPT_GNU 1 #define TEST_GETOPT_TMP_NAME "test-getopt-gnu.tmp" #include "test-getopt-main.h" gnuastro-0.5/bootstrapped/tests/test-getline.c0000644000175000017500000000463213217200023016554 00000000000000/* Test of getline() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (getline, ssize_t, (char **, size_t *, FILE *)); #include #include #include "macros.h" int main (void) { FILE *f; char *line; size_t len; ssize_t result; /* Create test file. */ f = fopen ("test-getline.txt", "wb"); if (!f || fwrite ("a\nA\nbc\nd\0f", 1, 10, f) != 10 || fclose (f) != 0) { fputs ("Failed to create sample file.\n", stderr); remove ("test-getline.txt"); return 1; } f = fopen ("test-getline.txt", "rb"); if (!f) { fputs ("Failed to reopen sample file.\n", stderr); remove ("test-getline.txt"); return 1; } /* Test initial allocation, which must include trailing NUL. */ line = NULL; len = 0; result = getline (&line, &len, f); ASSERT (result == 2); ASSERT (strcmp (line, "a\n") == 0); ASSERT (2 < len); free (line); /* Test initial allocation again, with line = NULL and len != 0. */ line = NULL; len = (size_t)(~0) / 4; result = getline (&line, &len, f); ASSERT (result == 2); ASSERT (strcmp (line, "A\n") == 0); ASSERT (2 < len); free (line); /* Test growth of buffer, must not leak. */ len = 1; line = malloc (len); result = getline (&line, &len, f); ASSERT (result == 3); ASSERT (strcmp (line, "bc\n") == 0); ASSERT (3 < len); /* Test embedded NULs and EOF behavior. */ result = getline (&line, &len, f); ASSERT (result == 3); ASSERT (memcmp (line, "d\0f", 4) == 0); ASSERT (3 < len); result = getline (&line, &len, f); ASSERT (result == -1); free (line); fclose (f); remove ("test-getline.txt"); return 0; } gnuastro-0.5/bootstrapped/tests/test-getdtablesize.c0000644000175000017500000000215113217200023017745 00000000000000/* Test of getdtablesize() function. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (getdtablesize, int, (void)); #include "macros.h" int main (int argc, char *argv[]) { ASSERT (getdtablesize () >= 3); ASSERT (dup2 (0, getdtablesize() - 1) == getdtablesize () - 1); ASSERT (dup2 (0, getdtablesize()) == -1); return 0; } gnuastro-0.5/bootstrapped/tests/test-getdelim.c0000644000175000017500000000465513217200023016724 00000000000000/* Test of getdelim() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake , 2007. */ #include #include #include "signature.h" SIGNATURE_CHECK (getdelim, ssize_t, (char **, size_t *, int, FILE *)); #include #include #include "macros.h" int main (void) { FILE *f; char *line; size_t len; ssize_t result; /* Create test file. */ f = fopen ("test-getdelim.txt", "wb"); if (!f || fwrite ("anAnbcnd\0f", 1, 10, f) != 10 || fclose (f) != 0) { fputs ("Failed to create sample file.\n", stderr); remove ("test-getdelim.txt"); return 1; } f = fopen ("test-getdelim.txt", "rb"); if (!f) { fputs ("Failed to reopen sample file.\n", stderr); remove ("test-getdelim.txt"); return 1; } /* Test initial allocation, which must include trailing NUL. */ line = NULL; len = 0; result = getdelim (&line, &len, 'n', f); ASSERT (result == 2); ASSERT (strcmp (line, "an") == 0); ASSERT (2 < len); free (line); /* Test initial allocation again, with line = NULL and len != 0. */ line = NULL; len = (size_t)(~0) / 4; result = getdelim (&line, &len, 'n', f); ASSERT (result == 2); ASSERT (strcmp (line, "An") == 0); ASSERT (2 < len); free (line); /* Test growth of buffer. */ line = malloc (1); len = 1; result = getdelim (&line, &len, 'n', f); ASSERT (result == 3); ASSERT (strcmp (line, "bcn") == 0); ASSERT (3 < len); /* Test embedded NULs and EOF behavior. */ result = getdelim (&line, &len, 'n', f); ASSERT (result == 3); ASSERT (memcmp (line, "d\0f", 4) == 0); ASSERT (3 < len); result = getdelim (&line, &len, 'n', f); ASSERT (result == -1); free (line); fclose (f); remove ("test-getdelim.txt"); return 0; } gnuastro-0.5/bootstrapped/tests/test-getcwd-lgpl.c0000644000175000017500000000510613217200023017333 00000000000000/* Test of getcwd() function. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (getcwd, char *, (char *, size_t)); #include #include #include #include #include "macros.h" int main (int argc, char **argv) { char *pwd1; char *pwd2; /* If the user provides an argument, attempt to chdir there first. */ if (1 < argc) { if (chdir (argv[1]) == 0) printf ("changed to directory %s\n", argv[1]); } pwd1 = getcwd (NULL, 0); ASSERT (pwd1 && *pwd1); if (1 < argc) printf ("cwd=%s\n", pwd1); /* Make sure the result is usable. */ ASSERT (chdir (pwd1) == 0); ASSERT (chdir (".//./.") == 0); /* Make sure that result is normalized. */ pwd2 = getcwd (NULL, 0); ASSERT (pwd2); ASSERT (strcmp (pwd1, pwd2) == 0); free (pwd2); { size_t len = strlen (pwd1); ssize_t i = len - 10; if (i < 1) i = 1; pwd2 = getcwd (NULL, len + 1); ASSERT (pwd2); free (pwd2); pwd2 = malloc (len + 2); for ( ; i <= len; i++) { char *tmp; errno = 0; ASSERT (getcwd (pwd2, i) == NULL); ASSERT (errno == ERANGE); /* Allow either glibc or BSD behavior, since POSIX allows both. */ errno = 0; tmp = getcwd (NULL, i); if (tmp) { ASSERT (strcmp (pwd1, tmp) == 0); free (tmp); } else { ASSERT (errno == ERANGE); } } ASSERT (getcwd (pwd2, len + 1) == pwd2); pwd2[len] = '/'; pwd2[len + 1] = '\0'; } ASSERT (strstr (pwd2, "/./") == NULL); ASSERT (strstr (pwd2, "/../") == NULL); ASSERT (strstr (pwd2 + 1 + (pwd2[1] == '/'), "//") == NULL); /* Validate a POSIX requirement on size. */ errno = 0; ASSERT (getcwd(pwd2, 0) == NULL); ASSERT (errno == EINVAL); free (pwd1); free (pwd2); return 0; } gnuastro-0.5/bootstrapped/tests/test-fwrite.c0000644000175000017500000000513113217200023016420 00000000000000/* Test of fwrite() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fwrite, size_t, (const void *, size_t, size_t, FILE *)); #include #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fwrite.txt"; /* We don't have an fwrite() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Test that fwrite() on an unbuffered stream sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "w"); char buf[5] = "world"; ASSERT (fp != NULL); setvbuf (fp, NULL, _IONBF, 0); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fwrite (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fwrite() on an unbuffered stream sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "w"); if (fp != NULL) { char buf[5] = "world"; setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fwrite (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "w"); if (fp != NULL) { char buf[5] = "world"; setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fwrite (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.5/bootstrapped/tests/test-func.c0000644000175000017500000000232413217200023016054 00000000000000/* Test whether __func__ is available Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "macros.h" int main () { ASSERT (strlen (__func__) > 0); /* On SunPRO C 5.9, sizeof __func__ evaluates to 0. The compiler warns: "warning: null dimension: sizeof()". */ #if !defined __SUNPRO_C ASSERT (strlen (__func__) + 1 == sizeof __func__); #endif ASSERT (strcmp (__func__, "main") == 0 || strcmp (__func__, "") == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-ftruncate.c0000644000175000017500000000301713217200023017114 00000000000000/* Test truncating a file. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (ftruncate, int, (int, off_t)); #include #include #include "macros.h" int main (int argc, char *argv[]) { const char *filename = argv[1]; /* Test behaviour for invalid file descriptors. */ { errno = 0; ASSERT (ftruncate (-1, 0) == -1); ASSERT (errno == EBADF); } { close (99); errno = 0; ASSERT (ftruncate (99, 0) == -1); ASSERT (errno == EBADF); } /* Test behaviour for read-only file descriptors. */ { int fd = open (filename, O_RDONLY); ASSERT (fd >= 0); errno = 0; ASSERT (ftruncate (fd, 0) == -1); ASSERT (errno == EBADF || errno == EINVAL || errno == EACCES /* seen on mingw */ ); close (fd); } return 0; } gnuastro-0.5/bootstrapped/tests/test-fstat.c0000644000175000017500000000237513217200023016250 00000000000000/* Tests of fstat() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fstat, int, (int, struct stat *)); #include #include #include "macros.h" int main (int argc, char *argv[]) { /* Test behaviour for invalid file descriptors. */ { struct stat statbuf; errno = 0; ASSERT (fstat (-1, &statbuf) == -1); ASSERT (errno == EBADF); } { struct stat statbuf; close (99); errno = 0; ASSERT (fstat (99, &statbuf) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.5/bootstrapped/tests/test-fread.c0000644000175000017500000000516113217200023016204 00000000000000/* Test of fread() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fread, size_t, (void *, size_t, size_t, FILE *)); #include #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fread.txt"; /* We don't have an fread() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Prepare a file. */ { const char text[] = "hello world"; int fd = open (filename, O_RDWR | O_CREAT | O_TRUNC, 0600); ASSERT (fd >= 0); ASSERT (write (fd, text, sizeof (text)) == sizeof (text)); ASSERT (close (fd) == 0); } /* Test that fread() sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "r"); char buf[5]; ASSERT (fp != NULL); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fread (buf, 1, sizeof (buf), fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fread() sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "r"); if (fp != NULL) { char buf[1]; errno = 0; ASSERT (fread (buf, 1, 1, fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "r"); if (fp != NULL) { char buf[1]; errno = 0; ASSERT (fread (buf, 1, 1, fp) == 0); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.5/bootstrapped/tests/test-fputc.c0000644000175000017500000000465613217200023016254 00000000000000/* Test of fputc() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fputc, int, (int, FILE *)); #include #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fputc.txt"; /* We don't have an fputc() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Test that fputc() on an unbuffered stream sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "w"); ASSERT (fp != NULL); setvbuf (fp, NULL, _IONBF, 0); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fputc ('x', fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fputc() on an unbuffered stream sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "w"); if (fp != NULL) { setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fputc ('x', fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "w"); if (fp != NULL) { setvbuf (fp, NULL, _IONBF, 0); errno = 0; ASSERT (fputc ('x', fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.5/bootstrapped/tests/test-float.c0000644000175000017500000002162513217200023016233 00000000000000/* Test of substitute. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2011. */ #include #include #include "fpucw.h" #include "macros.h" /* Check that FLT_RADIX is a constant expression. */ int a[] = { FLT_RADIX }; #if FLT_RADIX == 2 /* Return 2^n. */ static float pow2f (int n) { int k = n; volatile float x = 1; volatile float y = 2; /* Invariant: 2^n == x * y^k. */ if (k < 0) { y = 0.5f; k = - k; } while (k > 0) { if (k != 2 * (k / 2)) { x = x * y; k = k - 1; } if (k == 0) break; y = y * y; k = k / 2; } /* Now k == 0, hence x == 2^n. */ return x; } /* Return 2^n. */ static double pow2d (int n) { int k = n; volatile double x = 1; volatile double y = 2; /* Invariant: 2^n == x * y^k. */ if (k < 0) { y = 0.5; k = - k; } while (k > 0) { if (k != 2 * (k / 2)) { x = x * y; k = k - 1; } if (k == 0) break; y = y * y; k = k / 2; } /* Now k == 0, hence x == 2^n. */ return x; } /* Return 2^n. */ static long double pow2l (int n) { int k = n; volatile long double x = 1; volatile long double y = 2; /* Invariant: 2^n == x * y^k. */ if (k < 0) { y = 0.5L; k = - k; } while (k > 0) { if (k != 2 * (k / 2)) { x = x * y; k = k - 1; } if (k == 0) break; y = y * y; k = k / 2; } /* Now k == 0, hence x == 2^n. */ return x; } /* ----------------------- Check macros for 'float' ----------------------- */ /* Check that the FLT_* macros expand to constant expressions. */ int fb[] = { FLT_MANT_DIG, FLT_MIN_EXP, FLT_MAX_EXP, FLT_DIG, FLT_MIN_10_EXP, FLT_MAX_10_EXP }; float fc[] = { FLT_EPSILON, FLT_MIN, FLT_MAX }; static void test_float (void) { /* Check that the value of FLT_MIN_EXP is well parenthesized. */ ASSERT ((FLT_MIN_EXP % 101111) == (FLT_MIN_EXP) % 101111); /* Check that the value of DBL_MIN_10_EXP is well parenthesized. */ ASSERT ((FLT_MIN_10_EXP % 101111) == (FLT_MIN_10_EXP) % 101111); /* Check that 'float' is as specified in IEEE 754. */ ASSERT (FLT_MANT_DIG == 24); ASSERT (FLT_MIN_EXP == -125); ASSERT (FLT_MAX_EXP == 128); /* Check the value of FLT_MIN_10_EXP. */ ASSERT (FLT_MIN_10_EXP == - (int) (- (FLT_MIN_EXP - 1) * 0.30103)); /* Check the value of FLT_DIG. */ ASSERT (FLT_DIG == (int) ((FLT_MANT_DIG - 1) * 0.30103)); /* Check the value of FLT_MIN_10_EXP. */ ASSERT (FLT_MIN_10_EXP == - (int) (- (FLT_MIN_EXP - 1) * 0.30103)); /* Check the value of FLT_MAX_10_EXP. */ ASSERT (FLT_MAX_10_EXP == (int) (FLT_MAX_EXP * 0.30103)); /* Check the value of FLT_MAX. */ { volatile float m = FLT_MAX; int n; ASSERT (m + m > m); for (n = 0; n <= 2 * FLT_MANT_DIG; n++) { volatile float pow2_n = pow2f (n); /* 2^n */ volatile float x = m + (m / pow2_n); if (x > m) ASSERT (x + x == x); else ASSERT (!(x + x == x)); } } /* Check the value of FLT_MIN. */ { volatile float m = FLT_MIN; volatile float x = pow2f (FLT_MIN_EXP - 1); ASSERT (m == x); } /* Check the value of FLT_EPSILON. */ { volatile float e = FLT_EPSILON; volatile float me; int n; me = 1.0f + e; ASSERT (me > 1.0f); ASSERT (me - 1.0f == e); for (n = 0; n <= 2 * FLT_MANT_DIG; n++) { volatile float half_n = pow2f (- n); /* 2^-n */ volatile float x = me - half_n; if (x < me) ASSERT (x <= 1.0f); } } } /* ----------------------- Check macros for 'double' ----------------------- */ /* Check that the DBL_* macros expand to constant expressions. */ int db[] = { DBL_MANT_DIG, DBL_MIN_EXP, DBL_MAX_EXP, DBL_DIG, DBL_MIN_10_EXP, DBL_MAX_10_EXP }; double dc[] = { DBL_EPSILON, DBL_MIN, DBL_MAX }; static void test_double (void) { /* Check that the value of DBL_MIN_EXP is well parenthesized. */ ASSERT ((DBL_MIN_EXP % 101111) == (DBL_MIN_EXP) % 101111); /* Check that the value of DBL_MIN_10_EXP is well parenthesized. */ ASSERT ((DBL_MIN_10_EXP % 101111) == (DBL_MIN_10_EXP) % 101111); /* Check that 'double' is as specified in IEEE 754. */ ASSERT (DBL_MANT_DIG == 53); ASSERT (DBL_MIN_EXP == -1021); ASSERT (DBL_MAX_EXP == 1024); /* Check the value of DBL_MIN_10_EXP. */ ASSERT (DBL_MIN_10_EXP == - (int) (- (DBL_MIN_EXP - 1) * 0.30103)); /* Check the value of DBL_DIG. */ ASSERT (DBL_DIG == (int) ((DBL_MANT_DIG - 1) * 0.30103)); /* Check the value of DBL_MIN_10_EXP. */ ASSERT (DBL_MIN_10_EXP == - (int) (- (DBL_MIN_EXP - 1) * 0.30103)); /* Check the value of DBL_MAX_10_EXP. */ ASSERT (DBL_MAX_10_EXP == (int) (DBL_MAX_EXP * 0.30103)); /* Check the value of DBL_MAX. */ { volatile double m = DBL_MAX; int n; ASSERT (m + m > m); for (n = 0; n <= 2 * DBL_MANT_DIG; n++) { volatile double pow2_n = pow2d (n); /* 2^n */ volatile double x = m + (m / pow2_n); if (x > m) ASSERT (x + x == x); else ASSERT (!(x + x == x)); } } /* Check the value of DBL_MIN. */ { volatile double m = DBL_MIN; volatile double x = pow2d (DBL_MIN_EXP - 1); ASSERT (m == x); } /* Check the value of DBL_EPSILON. */ { volatile double e = DBL_EPSILON; volatile double me; int n; me = 1.0 + e; ASSERT (me > 1.0); ASSERT (me - 1.0 == e); for (n = 0; n <= 2 * DBL_MANT_DIG; n++) { volatile double half_n = pow2d (- n); /* 2^-n */ volatile double x = me - half_n; if (x < me) ASSERT (x <= 1.0); } } } /* -------------------- Check macros for 'long double' -------------------- */ /* Check that the LDBL_* macros expand to constant expressions. */ int lb[] = { LDBL_MANT_DIG, LDBL_MIN_EXP, LDBL_MAX_EXP, LDBL_DIG, LDBL_MIN_10_EXP, LDBL_MAX_10_EXP }; long double lc1 = LDBL_EPSILON; long double lc2 = LDBL_MIN; #if 0 /* LDBL_MAX is not a constant expression on some platforms. */ long double lc3 = LDBL_MAX; #endif static void test_long_double (void) { /* Check that the value of LDBL_MIN_EXP is well parenthesized. */ ASSERT ((LDBL_MIN_EXP % 101111) == (LDBL_MIN_EXP) % 101111); /* Check that the value of LDBL_MIN_10_EXP is well parenthesized. */ ASSERT ((LDBL_MIN_10_EXP % 101111) == (LDBL_MIN_10_EXP) % 101111); /* Check that 'long double' is at least as wide as 'double'. */ ASSERT (LDBL_MANT_DIG >= DBL_MANT_DIG); ASSERT (LDBL_MIN_EXP - LDBL_MANT_DIG <= DBL_MIN_EXP - DBL_MANT_DIG); ASSERT (LDBL_MAX_EXP >= DBL_MAX_EXP); /* Check the value of LDBL_DIG. */ ASSERT (LDBL_DIG == (int)((LDBL_MANT_DIG - 1) * 0.30103)); /* Check the value of LDBL_MIN_10_EXP. */ ASSERT (LDBL_MIN_10_EXP == - (int) (- (LDBL_MIN_EXP - 1) * 0.30103)); /* Check the value of LDBL_MAX_10_EXP. */ ASSERT (LDBL_MAX_10_EXP == (int) (LDBL_MAX_EXP * 0.30103)); /* Check the value of LDBL_MAX. */ { volatile long double m = LDBL_MAX; int n; ASSERT (m + m > m); for (n = 0; n <= 2 * LDBL_MANT_DIG; n++) { volatile long double pow2_n = pow2l (n); /* 2^n */ volatile long double x = m + (m / pow2_n); if (x > m) ASSERT (x + x == x); else ASSERT (!(x + x == x)); } } /* Check the value of LDBL_MIN. */ { volatile long double m = LDBL_MIN; volatile long double x = pow2l (LDBL_MIN_EXP - 1); ASSERT (m == x); } /* Check the value of LDBL_EPSILON. */ { volatile long double e = LDBL_EPSILON; volatile long double me; int n; me = 1.0L + e; ASSERT (me > 1.0L); ASSERT (me - 1.0L == e); for (n = 0; n <= 2 * LDBL_MANT_DIG; n++) { volatile long double half_n = pow2l (- n); /* 2^-n */ volatile long double x = me - half_n; if (x < me) ASSERT (x <= 1.0L); } } } int main () { test_float (); test_double (); { DECL_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING (); test_long_double (); END_LONG_DOUBLE_ROUNDING (); } return 0; } #else int main () { fprintf (stderr, "Skipping test: FLT_RADIX is not 2.\n"); return 77; } #endif gnuastro-0.5/bootstrapped/tests/test-fgetc.c0000644000175000017500000000476513217200023016224 00000000000000/* Test of fgetc() function. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fgetc, int, (FILE *)); #include #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #include "macros.h" int main (int argc, char **argv) { const char *filename = "test-fgetc.txt"; /* We don't have an fgetc() function that installs an invalid parameter handler so far. So install that handler here, explicitly. */ #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING gl_msvc_inval_ensure_handler (); #endif /* Prepare a file. */ { const char text[] = "hello world"; int fd = open (filename, O_RDWR | O_CREAT | O_TRUNC, 0600); ASSERT (fd >= 0); ASSERT (write (fd, text, sizeof (text)) == sizeof (text)); ASSERT (close (fd) == 0); } /* Test that fgetc() sets errno if someone else closes the stream fd behind the back of stdio. */ { FILE *fp = fopen (filename, "r"); ASSERT (fp != NULL); ASSERT (close (fileno (fp)) == 0); errno = 0; ASSERT (fgetc (fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } /* Test that fgetc() sets errno if the stream was constructed with an invalid file descriptor. */ { FILE *fp = fdopen (-1, "r"); if (fp != NULL) { errno = 0; ASSERT (fgetc (fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } { FILE *fp; close (99); fp = fdopen (99, "r"); if (fp != NULL) { errno = 0; ASSERT (fgetc (fp) == EOF); ASSERT (errno == EBADF); ASSERT (ferror (fp)); fclose (fp); } } /* Clean up. */ unlink (filename); return 0; } gnuastro-0.5/bootstrapped/tests/test-fdopen.c0000644000175000017500000000255713217200023016404 00000000000000/* Test opening a stream with a file descriptor. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (fdopen, FILE *, (int, const char *)); #include #include #include "macros.h" int main (void) { /* Test behavior on failure. POSIX makes it hard to check for failure, since the behavior is not well-defined on invalid file descriptors, so try fdopen 1000 times and if that's not enough to fail due to EMFILE, so be it. */ int i; for (i = 0; i < 1000; i++) { errno = 0; if (! fdopen (STDOUT_FILENO, "w")) { ASSERT (errno != 0); break; } } return 0; } gnuastro-0.5/bootstrapped/tests/test-fcntl-h.c0000644000175000017500000000552513217200023016462 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include /* Check that the various O_* macros are defined. */ int o = (O_DIRECT | O_DIRECTORY | O_DSYNC | O_IGNORE_CTTY | O_NDELAY | O_NOATIME | O_NONBLOCK | O_NOCTTY | O_NOFOLLOW | O_NOLINK | O_NOLINKS | O_NOTRANS | O_RSYNC | O_SYNC | O_TTY_INIT | O_BINARY | O_TEXT); /* Check that the various SEEK_* macros are defined. */ int sk[] = { SEEK_CUR, SEEK_END, SEEK_SET }; /* Check that the FD_* macros are defined. */ int i = FD_CLOEXEC; /* Check that the types are all defined. */ pid_t t1; off_t t2; mode_t t3; int main (void) { /* Ensure no overlap in SEEK_*. */ switch (0) { case SEEK_CUR: case SEEK_END: case SEEK_SET: ; } /* Ensure no dangerous overlap in non-zero gnulib-defined replacements. */ switch (O_RDONLY) { /* Access modes */ case O_RDONLY: case O_WRONLY: case O_RDWR: #if O_EXEC && O_EXEC != O_RDONLY case O_EXEC: #endif #if O_SEARCH && O_EXEC != O_SEARCH && O_SEARCH != O_RDONLY case O_SEARCH: #endif i = ! (~O_ACCMODE & (O_RDONLY | O_WRONLY | O_RDWR | O_EXEC | O_SEARCH)); break; /* Everyone should have these */ case O_CREAT: case O_EXCL: case O_TRUNC: case O_APPEND: break; /* These might be 0 or O_RDONLY, only test non-zero versions. */ #if O_CLOEXEC case O_CLOEXEC: #endif #if O_DIRECT case O_DIRECT: #endif #if O_DIRECTORY case O_DIRECTORY: #endif #if O_DSYNC case O_DSYNC: #endif #if O_IGNORE_CTTY case O_IGNORE_CTTY: #endif #if O_NOATIME case O_NOATIME: #endif #if O_NONBLOCK case O_NONBLOCK: #endif #if O_NOCTTY case O_NOCTTY: #endif #if O_NOFOLLOW case O_NOFOLLOW: #endif #if O_NOLINK case O_NOLINK: #endif #if O_NOLINKS case O_NOLINKS: #endif #if O_NOTRANS case O_NOTRANS: #endif #if O_RSYNC && O_RSYNC != O_DSYNC case O_RSYNC: #endif #if O_SYNC && O_SYNC != O_DSYNC && O_SYNC != O_RSYNC case O_SYNC: #endif #if O_TTY_INIT case O_TTY_INIT: #endif #if O_BINARY case O_BINARY: #endif #if O_TEXT case O_TEXT: #endif ; } return !i; } gnuastro-0.5/bootstrapped/tests/test-fcntl.c0000644000175000017500000002350613217200023016234 00000000000000/* Test of fcntl(2). Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include /* Specification. */ #include #include "signature.h" SIGNATURE_CHECK (fcntl, int, (int, int, ...)); /* Helpers. */ #include #include #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif #endif #include "binary-io.h" #include "macros.h" #if !O_BINARY # define setmode(f,m) zero () static int zero (void) { return 0; } #endif /* Return true if FD is open. */ static bool is_open (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ return (HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE; #else # ifndef F_GETFL # error Please port fcntl to your platform # endif return 0 <= fcntl (fd, F_GETFL); #endif } /* Return true if FD is open and inheritable across exec/spawn. */ static bool is_inheritable (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ HANDLE h = (HANDLE) _get_osfhandle (fd); DWORD flags; if (h == INVALID_HANDLE_VALUE || GetHandleInformation (h, &flags) == 0) return false; return (flags & HANDLE_FLAG_INHERIT) != 0; #else # ifndef F_GETFD # error Please port fcntl to your platform # endif int i = fcntl (fd, F_GETFD); return 0 <= i && (i & FD_CLOEXEC) == 0; #endif } /* Return non-zero if FD is open in the given MODE, which is either O_TEXT or O_BINARY. */ static bool is_mode (int fd, int mode) { int value = setmode (fd, O_BINARY); setmode (fd, value); return mode == value; } /* Since native fcntl can have more supported operations than our replacement is aware of, and since various operations assign different types to the vararg argument, a wrapper around fcntl must be able to pass a vararg of unknown type on through to the original fcntl. Make sure that this works properly: func1 behaves like the original fcntl interpreting the vararg as an int or a pointer to a struct, and func2 behaves like rpl_fcntl that doesn't know what type to forward. */ struct dummy_struct { long filler; int value; }; static int func1 (int a, ...) { va_list arg; int i; va_start (arg, a); if (a < 4) i = va_arg (arg, int); else { struct dummy_struct *s = va_arg (arg, struct dummy_struct *); i = s->value; } va_end (arg); return i; } static int func2 (int a, ...) { va_list arg; void *p; va_start (arg, a); p = va_arg (arg, void *); va_end (arg); return func1 (a, p); } /* Ensure that all supported fcntl actions are distinct, and usable in preprocessor expressions. */ static void check_flags (void) { switch (0) { case F_DUPFD: #if F_DUPFD #endif case F_DUPFD_CLOEXEC: #if F_DUPFD_CLOEXEC #endif case F_GETFD: #if F_GETFD #endif #ifdef F_SETFD case F_SETFD: # if F_SETFD # endif #endif #ifdef F_GETFL case F_GETFL: # if F_GETFL # endif #endif #ifdef F_SETFL case F_SETFL: # if F_SETFL # endif #endif #ifdef F_GETOWN case F_GETOWN: # if F_GETOWN # endif #endif #ifdef F_SETOWN case F_SETOWN: # if F_SETOWN # endif #endif #ifdef F_GETLK case F_GETLK: # if F_GETLK # endif #endif #ifdef F_SETLK case F_SETLK: # if F_SETLK # endif #endif #ifdef F_SETLKW case F_SETLKW: # if F_SETLKW # endif #endif ; } } int main (void) { const char *file = "test-fcntl.tmp"; int fd; int bad_fd = getdtablesize (); /* Sanity check that rpl_fcntl is likely to work. */ ASSERT (func2 (1, 2) == 2); ASSERT (func2 (2, -2) == -2); ASSERT (func2 (3, 0x80000000) == 0x80000000); { struct dummy_struct s = { 0L, 4 }; ASSERT (func2 (4, &s) == 4); } check_flags (); /* Assume std descriptors were provided by invoker, and ignore fds that might have been inherited. */ fd = creat (file, 0600); ASSERT (STDERR_FILENO < fd); close (fd + 1); close (fd + 2); /* For F_DUPFD*, the source must be valid. */ errno = 0; ASSERT (fcntl (-1, F_DUPFD, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_DUPFD, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_DUPFD, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (-1, F_DUPFD_CLOEXEC, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_DUPFD_CLOEXEC, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_DUPFD_CLOEXEC, 0) == -1); ASSERT (errno == EBADF); /* For F_DUPFD*, the destination must be valid. */ errno = 0; ASSERT (fcntl (fd, F_DUPFD, -1) == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (fcntl (fd, F_DUPFD, bad_fd) == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (fcntl (fd, F_DUPFD_CLOEXEC, -1) == -1); ASSERT (errno == EINVAL); errno = 0; ASSERT (fcntl (fd, F_DUPFD_CLOEXEC, bad_fd) == -1); ASSERT (errno == EINVAL); /* For F_DUPFD*, check for correct inheritance, as well as preservation of text vs. binary. */ setmode (fd, O_BINARY); ASSERT (is_open (fd)); ASSERT (!is_open (fd + 1)); ASSERT (!is_open (fd + 2)); ASSERT (is_inheritable (fd)); ASSERT (is_mode (fd, O_BINARY)); ASSERT (fcntl (fd, F_DUPFD, fd) == fd + 1); ASSERT (is_open (fd)); ASSERT (is_open (fd + 1)); ASSERT (!is_open (fd + 2)); ASSERT (is_inheritable (fd + 1)); ASSERT (is_mode (fd, O_BINARY)); ASSERT (is_mode (fd + 1, O_BINARY)); ASSERT (close (fd + 1) == 0); ASSERT (fcntl (fd, F_DUPFD_CLOEXEC, fd + 2) == fd + 2); ASSERT (is_open (fd)); ASSERT (!is_open (fd + 1)); ASSERT (is_open (fd + 2)); ASSERT (is_inheritable (fd)); ASSERT (!is_inheritable (fd + 2)); ASSERT (is_mode (fd, O_BINARY)); ASSERT (is_mode (fd + 2, O_BINARY)); ASSERT (close (fd) == 0); setmode (fd + 2, O_TEXT); ASSERT (fcntl (fd + 2, F_DUPFD, fd + 1) == fd + 1); ASSERT (!is_open (fd)); ASSERT (is_open (fd + 1)); ASSERT (is_open (fd + 2)); ASSERT (is_inheritable (fd + 1)); ASSERT (!is_inheritable (fd + 2)); ASSERT (is_mode (fd + 1, O_TEXT)); ASSERT (is_mode (fd + 2, O_TEXT)); ASSERT (close (fd + 1) == 0); ASSERT (fcntl (fd + 2, F_DUPFD_CLOEXEC, 0) == fd); ASSERT (is_open (fd)); ASSERT (!is_open (fd + 1)); ASSERT (is_open (fd + 2)); ASSERT (!is_inheritable (fd)); ASSERT (!is_inheritable (fd + 2)); ASSERT (is_mode (fd, O_TEXT)); ASSERT (is_mode (fd + 2, O_TEXT)); ASSERT (close (fd + 2) == 0); /* Test F_GETFD on invalid file descriptors. */ errno = 0; ASSERT (fcntl (-1, F_GETFD) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_GETFD) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_GETFD) == -1); ASSERT (errno == EBADF); /* Test F_GETFD, the FD_CLOEXEC bit. */ { int result = fcntl (fd, F_GETFD); ASSERT (0 <= result); ASSERT ((result & FD_CLOEXEC) == FD_CLOEXEC); ASSERT (dup (fd) == fd + 1); result = fcntl (fd + 1, F_GETFD); ASSERT (0 <= result); ASSERT ((result & FD_CLOEXEC) == 0); ASSERT (close (fd + 1) == 0); } #ifdef F_SETFD /* Test F_SETFD on invalid file descriptors. */ errno = 0; ASSERT (fcntl (-1, F_SETFD, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_SETFD, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_SETFD, 0) == -1); ASSERT (errno == EBADF); #endif #ifdef F_GETFL /* Test F_GETFL on invalid file descriptors. */ errno = 0; ASSERT (fcntl (-1, F_GETFL) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_GETFL) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_GETFL) == -1); ASSERT (errno == EBADF); #endif #ifdef F_SETFL /* Test F_SETFL on invalid file descriptors. */ errno = 0; ASSERT (fcntl (-1, F_SETFL, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_SETFL, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_SETFL, 0) == -1); ASSERT (errno == EBADF); #endif #ifdef F_GETOWN /* Test F_GETOWN on invalid file descriptors. */ errno = 0; ASSERT (fcntl (-1, F_GETOWN) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_GETOWN) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_GETOWN) == -1); ASSERT (errno == EBADF); #endif #ifdef F_SETOWN /* Test F_SETFL on invalid file descriptors. */ errno = 0; ASSERT (fcntl (-1, F_SETOWN, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (fd + 1, F_SETOWN, 0) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (fcntl (bad_fd, F_SETOWN, 0) == -1); ASSERT (errno == EBADF); #endif /* Cleanup. */ ASSERT (close (fd) == 0); ASSERT (unlink (file) == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-errno.c0000644000175000017500000000555513217200023016257 00000000000000/* Test of substitute. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include /* Verify that the POSIX mandated errno values exist and can be used as initializers outside of a function. The variable names happen to match the Linux/x86 error numbers. */ int e1 = EPERM; int e2 = ENOENT; int e3 = ESRCH; int e4 = EINTR; int e5 = EIO; int e6 = ENXIO; int e7 = E2BIG; int e8 = ENOEXEC; int e9 = EBADF; int e10 = ECHILD; int e11 = EAGAIN; int e11a = EWOULDBLOCK; int e12 = ENOMEM; int e13 = EACCES; int e14 = EFAULT; int e16 = EBUSY; int e17 = EEXIST; int e18 = EXDEV; int e19 = ENODEV; int e20 = ENOTDIR; int e21 = EISDIR; int e22 = EINVAL; int e23 = ENFILE; int e24 = EMFILE; int e25 = ENOTTY; int e26 = ETXTBSY; int e27 = EFBIG; int e28 = ENOSPC; int e29 = ESPIPE; int e30 = EROFS; int e31 = EMLINK; int e32 = EPIPE; int e33 = EDOM; int e34 = ERANGE; int e35 = EDEADLK; int e36 = ENAMETOOLONG; int e37 = ENOLCK; int e38 = ENOSYS; int e39 = ENOTEMPTY; int e40 = ELOOP; int e42 = ENOMSG; int e43 = EIDRM; int e67 = ENOLINK; int e71 = EPROTO; int e72 = EMULTIHOP; int e74 = EBADMSG; int e75 = EOVERFLOW; int e84 = EILSEQ; int e88 = ENOTSOCK; int e89 = EDESTADDRREQ; int e90 = EMSGSIZE; int e91 = EPROTOTYPE; int e92 = ENOPROTOOPT; int e93 = EPROTONOSUPPORT; int e95 = EOPNOTSUPP; int e95a = ENOTSUP; int e97 = EAFNOSUPPORT; int e98 = EADDRINUSE; int e99 = EADDRNOTAVAIL; int e100 = ENETDOWN; int e101 = ENETUNREACH; int e102 = ENETRESET; int e103 = ECONNABORTED; int e104 = ECONNRESET; int e105 = ENOBUFS; int e106 = EISCONN; int e107 = ENOTCONN; int e110 = ETIMEDOUT; int e111 = ECONNREFUSED; int e113 = EHOSTUNREACH; int e114 = EALREADY; int e115 = EINPROGRESS; int e116 = ESTALE; int e122 = EDQUOT; int e125 = ECANCELED; int e130 = EOWNERDEAD; int e131 = ENOTRECOVERABLE; /* Don't verify that these errno values are all different, except for possibly EWOULDBLOCK == EAGAIN. Even Linux/x86 does not pass this check: it has ENOTSUP == EOPNOTSUPP. */ int main () { /* Verify that errno can be assigned. */ errno = EOVERFLOW; /* snprintf() callers want to distinguish EINVAL and EOVERFLOW. */ if (errno == EINVAL) return 1; return 0; } gnuastro-0.5/bootstrapped/tests/test-environ.c0000644000175000017500000000273013217200023016602 00000000000000/* Test of environ variable. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include int main () { /* The environment variables that are set even in the weirdest situations are HOME and PATH. POSIX says that HOME is initialized by the system, and that PATH may be unset. But in practice it's more frequent to see HOME unset and PATH set. So we test the presence of PATH. */ char **remaining_variables = environ; char *string; for (; (string = *remaining_variables) != NULL; remaining_variables++) { if (strncmp (string, "PATH=", 5) == 0) /* Found the PATH environment variable. */ return 0; } /* Failed to find the PATH environment variable. */ return 1; } gnuastro-0.5/bootstrapped/tests/test-dup2.c0000644000175000017500000001406213217200023015775 00000000000000/* Test duplicating file descriptors. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include #include "signature.h" SIGNATURE_CHECK (dup2, int, (int, int)); #include #include #if HAVE_SYS_RESOURCE_H # include #endif #include "binary-io.h" #if GNULIB_TEST_CLOEXEC # include "cloexec.h" #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif #endif #include "macros.h" /* Return non-zero if FD is open. */ static int is_open (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ return (HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE; #else # ifndef F_GETFL # error Please port fcntl to your platform # endif return 0 <= fcntl (fd, F_GETFL); #endif } #if GNULIB_TEST_CLOEXEC /* Return non-zero if FD is open and inheritable across exec/spawn. */ static int is_inheritable (int fd) { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ HANDLE h = (HANDLE) _get_osfhandle (fd); DWORD flags; if (h == INVALID_HANDLE_VALUE || GetHandleInformation (h, &flags) == 0) return 0; return (flags & HANDLE_FLAG_INHERIT) != 0; # else # ifndef F_GETFD # error Please port fcntl to your platform # endif int i = fcntl (fd, F_GETFD); return 0 <= i && (i & FD_CLOEXEC) == 0; # endif } #endif /* GNULIB_TEST_CLOEXEC */ #if !O_BINARY # define setmode(f,m) zero () static int zero (void) { return 0; } #endif /* Return non-zero if FD is open in the given MODE, which is either O_TEXT or O_BINARY. */ static int is_mode (int fd, int mode) { int value = setmode (fd, O_BINARY); setmode (fd, value); return mode == value; } int main (void) { const char *file = "test-dup2.tmp"; char buffer[1]; int bad_fd = getdtablesize (); int fd = open (file, O_CREAT | O_TRUNC | O_RDWR, 0600); /* Assume std descriptors were provided by invoker. */ ASSERT (STDERR_FILENO < fd); ASSERT (is_open (fd)); /* Ignore any other fd's leaked into this process. */ close (fd + 1); close (fd + 2); ASSERT (!is_open (fd + 1)); ASSERT (!is_open (fd + 2)); /* Assigning to self must be a no-op. */ ASSERT (dup2 (fd, fd) == fd); ASSERT (is_open (fd)); /* The source must be valid. */ errno = 0; ASSERT (dup2 (-1, fd) == -1); ASSERT (errno == EBADF); close (99); errno = 0; ASSERT (dup2 (99, fd) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (dup2 (AT_FDCWD, fd) == -1); ASSERT (errno == EBADF); ASSERT (is_open (fd)); /* If the source is not open, then the destination is unaffected. */ errno = 0; ASSERT (dup2 (fd + 1, fd + 1) == -1); ASSERT (errno == EBADF); ASSERT (!is_open (fd + 1)); errno = 0; ASSERT (dup2 (fd + 1, fd) == -1); ASSERT (errno == EBADF); ASSERT (is_open (fd)); /* The destination must be valid. */ errno = 0; ASSERT (dup2 (fd, -2) == -1); ASSERT (errno == EBADF); if (bad_fd > 256) { ASSERT (dup2 (fd, 255) == 255); ASSERT (dup2 (fd, 256) == 256); ASSERT (close (255) == 0); ASSERT (close (256) == 0); } ASSERT (dup2 (fd, bad_fd - 1) == bad_fd - 1); ASSERT (close (bad_fd - 1) == 0); errno = 0; ASSERT (dup2 (fd, bad_fd) == -1); ASSERT (errno == EBADF); /* Using dup2 can skip fds. */ ASSERT (dup2 (fd, fd + 2) == fd + 2); ASSERT (is_open (fd)); ASSERT (!is_open (fd + 1)); ASSERT (is_open (fd + 2)); /* Verify that dup2 closes the previous occupant of a fd. */ ASSERT (open ("/dev/null", O_WRONLY, 0600) == fd + 1); ASSERT (dup2 (fd + 1, fd) == fd); ASSERT (close (fd + 1) == 0); ASSERT (write (fd, "1", 1) == 1); ASSERT (dup2 (fd + 2, fd) == fd); ASSERT (lseek (fd, 0, SEEK_END) == 0); ASSERT (write (fd + 2, "2", 1) == 1); ASSERT (lseek (fd, 0, SEEK_SET) == 0); ASSERT (read (fd, buffer, 1) == 1); ASSERT (*buffer == '2'); #if GNULIB_TEST_CLOEXEC /* Any new fd created by dup2 must not be cloexec. */ ASSERT (close (fd + 2) == 0); ASSERT (dup_cloexec (fd) == fd + 1); ASSERT (!is_inheritable (fd + 1)); ASSERT (dup2 (fd + 1, fd + 1) == fd + 1); ASSERT (!is_inheritable (fd + 1)); ASSERT (dup2 (fd + 1, fd + 2) == fd + 2); ASSERT (!is_inheritable (fd + 1)); ASSERT (is_inheritable (fd + 2)); errno = 0; ASSERT (dup2 (fd + 1, -1) == -1); ASSERT (errno == EBADF); ASSERT (!is_inheritable (fd + 1)); #endif /* On systems that distinguish between text and binary mode, dup2 reuses the mode of the source. */ setmode (fd, O_BINARY); ASSERT (is_mode (fd, O_BINARY)); ASSERT (dup2 (fd, fd + 1) == fd + 1); ASSERT (is_mode (fd + 1, O_BINARY)); setmode (fd, O_TEXT); ASSERT (is_mode (fd, O_TEXT)); ASSERT (dup2 (fd, fd + 1) == fd + 1); ASSERT (is_mode (fd + 1, O_TEXT)); /* Clean up. */ ASSERT (close (fd + 2) == 0); ASSERT (close (fd + 1) == 0); ASSERT (close (fd) == 0); ASSERT (unlink (file) == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-ctype.c0000644000175000017500000000154113217200023016245 00000000000000/* Test of substitute. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-connect.c0000644000175000017500000000314313217200023016552 00000000000000/* Test connecting a client socket. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (connect, int, (int, const struct sockaddr *, socklen_t)); #include #include #include #include #include "sockets.h" #include "macros.h" int main (void) { (void) gl_sockets_startup (SOCKETS_1_1); /* Test behaviour for invalid file descriptors. */ { struct sockaddr_in addr; addr.sin_family = AF_INET; inet_pton (AF_INET, "127.0.0.1", &addr.sin_addr); addr.sin_port = htons (80); { errno = 0; ASSERT (connect (-1, (const struct sockaddr *) &addr, sizeof (addr)) == -1); ASSERT (errno == EBADF); } { close (99); errno = 0; ASSERT (connect (99, (const struct sockaddr *) &addr, sizeof (addr)) == -1); ASSERT (errno == EBADF); } } return 0; } gnuastro-0.5/bootstrapped/tests/test-close.c0000644000175000017500000000220213217200023016221 00000000000000/* Test closing a file or socket. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (close, int, (int)); #include #include "macros.h" int main (void) { /* Test behaviour for invalid file descriptors. */ { errno = 0; ASSERT (close (-1) == -1); ASSERT (errno == EBADF); } { close (99); errno = 0; ASSERT (close (99) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.5/bootstrapped/tests/test-cloexec.c0000644000175000017500000001003413217200023016540 00000000000000/* Test duplicating non-inheritable file descriptors. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake , 2009. */ #include #include "cloexec.h" #include #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif #endif #include "binary-io.h" #include "macros.h" /* Return non-zero if FD is open and inheritable across exec/spawn. */ static int is_inheritable (int fd) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, the initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE, and there is no fcntl. */ HANDLE h = (HANDLE) _get_osfhandle (fd); DWORD flags; if (h == INVALID_HANDLE_VALUE || GetHandleInformation (h, &flags) == 0) return 0; return (flags & HANDLE_FLAG_INHERIT) != 0; #else # ifndef F_GETFD # error Please port fcntl to your platform # endif int i = fcntl (fd, F_GETFD); return 0 <= i && (i & FD_CLOEXEC) == 0; #endif } #if !O_BINARY # define setmode(f,m) zero () static int zero (void) { return 0; } #endif /* Return non-zero if FD is open in the given MODE, which is either O_TEXT or O_BINARY. */ static int is_mode (int fd, int mode) { int value = setmode (fd, O_BINARY); setmode (fd, value); return mode == value; } int main (void) { const char *file = "test-cloexec.tmp"; int fd = creat (file, 0600); int fd2; int bad_fd = getdtablesize (); /* Assume std descriptors were provided by invoker. */ ASSERT (STDERR_FILENO < fd); ASSERT (is_inheritable (fd)); /* Normal use of set_cloexec_flag. */ ASSERT (set_cloexec_flag (fd, true) == 0); #if !((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) ASSERT (!is_inheritable (fd)); #endif ASSERT (set_cloexec_flag (fd, false) == 0); ASSERT (is_inheritable (fd)); /* Normal use of dup_cloexec. */ fd2 = dup_cloexec (fd); ASSERT (fd < fd2); ASSERT (!is_inheritable (fd2)); ASSERT (close (fd) == 0); ASSERT (dup_cloexec (fd2) == fd); ASSERT (!is_inheritable (fd)); ASSERT (close (fd2) == 0); /* On systems that distinguish between text and binary mode, dup_cloexec reuses the mode of the source. */ setmode (fd, O_BINARY); ASSERT (is_mode (fd, O_BINARY)); fd2 = dup_cloexec (fd); ASSERT (fd < fd2); ASSERT (is_mode (fd2, O_BINARY)); ASSERT (close (fd2) == 0); setmode (fd, O_TEXT); ASSERT (is_mode (fd, O_TEXT)); fd2 = dup_cloexec (fd); ASSERT (fd < fd2); ASSERT (is_mode (fd2, O_TEXT)); ASSERT (close (fd2) == 0); /* Test error handling. */ errno = 0; ASSERT (set_cloexec_flag (-1, false) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (set_cloexec_flag (bad_fd, false) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (set_cloexec_flag (fd2, false) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (dup_cloexec (-1) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (dup_cloexec (bad_fd) == -1); ASSERT (errno == EBADF); errno = 0; ASSERT (dup_cloexec (fd2) == -1); ASSERT (errno == EBADF); /* Clean up. */ ASSERT (close (fd) == 0); ASSERT (unlink (file) == 0); return 0; } gnuastro-0.5/bootstrapped/tests/test-c-strncasecmp.c0000644000175000017500000000601113217200023017660 00000000000000/* Test of case-insensitive string comparison function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "c-strcase.h" #include "c-ctype.h" #include #include #include "macros.h" int main (int argc, char *argv[]) { if (argc > 1) { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; } ASSERT (c_strncasecmp ("paragraph", "Paragraph", 1000000) == 0); ASSERT (c_strncasecmp ("paragraph", "Paragraph", 9) == 0); ASSERT (c_strncasecmp ("paragrapH", "parAgRaph", 1000000) == 0); ASSERT (c_strncasecmp ("paragrapH", "parAgRaph", 9) == 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 10) < 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 9) < 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 5) < 0); ASSERT (c_strncasecmp ("paragraph", "paraLyzed", 4) == 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 10) > 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 9) > 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 5) > 0); ASSERT (c_strncasecmp ("paraLyzed", "paragraph", 4) == 0); ASSERT (c_strncasecmp ("para", "paragraph", 10) < 0); ASSERT (c_strncasecmp ("para", "paragraph", 9) < 0); ASSERT (c_strncasecmp ("para", "paragraph", 5) < 0); ASSERT (c_strncasecmp ("para", "paragraph", 4) == 0); ASSERT (c_strncasecmp ("paragraph", "para", 10) > 0); ASSERT (c_strncasecmp ("paragraph", "para", 9) > 0); ASSERT (c_strncasecmp ("paragraph", "para", 5) > 0); ASSERT (c_strncasecmp ("paragraph", "para", 4) == 0); /* The following tests shows how c_strncasecmp() is different from strncasecmp(). */ ASSERT (c_strncasecmp ("\311mily", "\351mile", 4) < 0); ASSERT (c_strncasecmp ("\351mile", "\311mily", 4) > 0); /* The following tests shows how c_strncasecmp() is different from mbsncasecmp(). */ ASSERT (c_strncasecmp ("\303\266zg\303\274r", "\303\226ZG\303\234R", 99) > 0); /* özgür */ ASSERT (c_strncasecmp ("\303\226ZG\303\234R", "\303\266zg\303\274r", 99) < 0); /* özgür */ #if C_CTYPE_ASCII /* This test shows how strings of different size cannot compare equal. */ ASSERT (c_strncasecmp ("turkish", "TURK\304\260SH", 7) < 0); ASSERT (c_strncasecmp ("TURK\304\260SH", "turkish", 7) > 0); #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-c-strcasecmp.c0000644000175000017500000000422313217200023017505 00000000000000/* Test of case-insensitive string comparison function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "c-strcase.h" #include "c-ctype.h" #include #include #include "macros.h" int main (int argc, char *argv[]) { if (argc > 1) { /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; } ASSERT (c_strcasecmp ("paragraph", "Paragraph") == 0); ASSERT (c_strcasecmp ("paragrapH", "parAgRaph") == 0); ASSERT (c_strcasecmp ("paragraph", "paraLyzed") < 0); ASSERT (c_strcasecmp ("paraLyzed", "paragraph") > 0); ASSERT (c_strcasecmp ("para", "paragraph") < 0); ASSERT (c_strcasecmp ("paragraph", "para") > 0); /* The following tests shows how c_strcasecmp() is different from strcasecmp(). */ ASSERT (c_strcasecmp ("\311mile", "\351mile") < 0); ASSERT (c_strcasecmp ("\351mile", "\311mile") > 0); /* The following tests shows how c_strcasecmp() is different from mbscasecmp(). */ ASSERT (c_strcasecmp ("\303\266zg\303\274r", "\303\226ZG\303\234R") > 0); /* özgür */ ASSERT (c_strcasecmp ("\303\226ZG\303\234R", "\303\266zg\303\274r") < 0); /* özgür */ #if C_CTYPE_ASCII /* This test shows how strings of different size cannot compare equal. */ ASSERT (c_strcasecmp ("turkish", "TURK\304\260SH") < 0); ASSERT (c_strcasecmp ("TURK\304\260SH", "turkish") > 0); #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-c-ctype.c0000644000175000017500000001464413217200023016475 00000000000000/* Test of character handling in C locale. Copyright (C) 2005, 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #include "c-ctype.h" #include #include #include #include "macros.h" static void test_agree_with_C_locale (void) { int c; for (c = 0; c <= UCHAR_MAX; c++) { ASSERT (c_isascii (c) == (isascii (c) != 0)); if (c_isascii (c)) { ASSERT (c_isalnum (c) == (isalnum (c) != 0)); ASSERT (c_isalpha (c) == (isalpha (c) != 0)); ASSERT (c_isblank (c) == (isblank (c) != 0)); ASSERT (c_iscntrl (c) == (iscntrl (c) != 0)); ASSERT (c_isdigit (c) == (isdigit (c) != 0)); ASSERT (c_islower (c) == (islower (c) != 0)); ASSERT (c_isgraph (c) == (isgraph (c) != 0)); ASSERT (c_isprint (c) == (isprint (c) != 0)); ASSERT (c_ispunct (c) == (ispunct (c) != 0)); ASSERT (c_isspace (c) == (isspace (c) != 0)); ASSERT (c_isupper (c) == (isupper (c) != 0)); ASSERT (c_isxdigit (c) == (isxdigit (c) != 0)); ASSERT (c_tolower (c) == tolower (c)); ASSERT (c_toupper (c) == toupper (c)); } } } static void test_all (void) { int c; int n_isascii = 0; for (c = CHAR_MIN; c <= UCHAR_MAX; c++) { if (! (0 <= c && c <= CHAR_MAX)) { ASSERT (! c_isascii (c)); ASSERT (! c_isalnum (c)); ASSERT (! c_isalpha (c)); ASSERT (! c_isblank (c)); ASSERT (! c_iscntrl (c)); ASSERT (! c_isdigit (c)); ASSERT (! c_islower (c)); ASSERT (! c_isgraph (c)); ASSERT (! c_isprint (c)); ASSERT (! c_ispunct (c)); ASSERT (! c_isspace (c)); ASSERT (! c_isupper (c)); ASSERT (! c_isxdigit (c)); ASSERT (c_tolower (c) == c); ASSERT (c_toupper (c) == c); } n_isascii += c_isascii (c); #ifdef C_CTYPE_ASCII ASSERT (c_isascii (c) == (0 <= c && c <= 0x7f)); #endif ASSERT (c_isascii (c) == (c_isprint (c) || c_iscntrl (c))); ASSERT (c_isalnum (c) == (c_isalpha (c) || c_isdigit (c))); ASSERT (c_isalpha (c) == (c_islower (c) || c_isupper (c))); switch (c) { case '\t': case ' ': ASSERT (c_isblank (c) == 1); break; default: ASSERT (c_isblank (c) == 0); break; } #ifdef C_CTYPE_ASCII ASSERT (c_iscntrl (c) == ((c >= 0 && c < 0x20) || c == 0x7f)); #endif switch (c) { case '\a': case '\b': case '\f': case '\n': case '\r': case '\t': case '\v': ASSERT (c_iscntrl (c)); break; } ASSERT (! (c_iscntrl (c) && c_isprint (c))); switch (c) { case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': ASSERT (c_isdigit (c) == 1); break; default: ASSERT (c_isdigit (c) == 0); break; } switch (c) { case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': ASSERT (c_islower (c) == 1); ASSERT (c_toupper (c) == c - 'a' + 'A'); break; default: ASSERT (c_islower (c) == 0); ASSERT (c_toupper (c) == c); break; } #ifdef C_CTYPE_ASCII ASSERT (c_isgraph (c) == ((c >= 0x20 && c < 0x7f) && c != ' ')); ASSERT (c_isprint (c) == (c >= 0x20 && c < 0x7f)); #endif ASSERT (c_isgraph (c) == (c_isalnum (c) || c_ispunct (c))); ASSERT (c_isprint (c) == (c_isgraph (c) || c == ' ')); switch (c) { case '!': case '"': case '#': case '$': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case ':': case ';': case '<': case '=': case '>': case '?': case '@': case '[': case'\\': case ']': case '^': case '_': case '`': case '{': case '|': case '}': case '~': ASSERT (c_ispunct (c) == 1); break; default: ASSERT (c_ispunct (c) == 0); break; } switch (c) { case ' ': case '\t': case '\n': case '\v': case '\f': case '\r': ASSERT (c_isspace (c) == 1); break; default: ASSERT (c_isspace (c) == 0); break; } switch (c) { case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': ASSERT (c_isupper (c) == 1); ASSERT (c_tolower (c) == c - 'A' + 'a'); break; default: ASSERT (c_isupper (c) == 0); ASSERT (c_tolower (c) == c); break; } switch (c) { case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': ASSERT (c_isxdigit (c) == 1); break; default: ASSERT (c_isxdigit (c) == 0); break; } } ASSERT (n_isascii == 128); } int main () { test_agree_with_C_locale (); test_all (); setlocale (LC_ALL, "de_DE"); test_all (); setlocale (LC_ALL, "ja_JP.EUC-JP"); test_all (); return 0; } gnuastro-0.5/bootstrapped/tests/test-btowc.c0000644000175000017500000000331113217200023016234 00000000000000/* Test of conversion of unibyte character to wide character. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include #include "signature.h" SIGNATURE_CHECK (btowc, wint_t, (int)); #include #include #include "macros.h" int main (int argc, char *argv[]) { int c; /* configure should already have checked that the locale is supported. */ if (setlocale (LC_ALL, "") == NULL) return 1; ASSERT (btowc (EOF) == WEOF); if (argc > 1) switch (argv[1][0]) { case '1': /* Locale encoding is ISO-8859-1 or ISO-8859-15. */ for (c = 0; c < 0x80; c++) ASSERT (btowc (c) == c); for (c = 0xA0; c < 0x100; c++) ASSERT (btowc (c) != WEOF); return 0; case '2': /* Locale encoding is UTF-8. */ for (c = 0; c < 0x80; c++) ASSERT (btowc (c) == c); for (c = 0x80; c < 0x100; c++) ASSERT (btowc (c) == WEOF); return 0; } return 1; } gnuastro-0.5/bootstrapped/tests/test-bind.c0000644000175000017500000000310513217200023016033 00000000000000/* Test binding a server socket to a port. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (bind, int, (int, const struct sockaddr *, socklen_t)); #include #include #include #include #include "sockets.h" #include "macros.h" int main (void) { (void) gl_sockets_startup (SOCKETS_1_1); /* Test behaviour for invalid file descriptors. */ { struct sockaddr_in addr; addr.sin_family = AF_INET; inet_pton (AF_INET, "127.0.0.1", &addr.sin_addr); addr.sin_port = htons (80); { errno = 0; ASSERT (bind (-1, (const struct sockaddr *) &addr, sizeof (addr)) == -1); ASSERT (errno == EBADF); } { close (99); errno = 0; ASSERT (bind (99, (const struct sockaddr *) &addr, sizeof (addr)) == -1); ASSERT (errno == EBADF); } } return 0; } gnuastro-0.5/bootstrapped/tests/test-binary-io.c0000644000175000017500000000305413217200023017013 00000000000000/* Test of binary mode I/O. Copyright (C) 2005, 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2005. */ #include #include "binary-io.h" #include #include #include #include #include #include #include "macros.h" int main (int argc, char *argv[]) { /* Test the O_BINARY macro. */ { int fd = open ("t-bin-out0.tmp", O_CREAT | O_TRUNC | O_RDWR | O_BINARY, 0600); if (write (fd, "Hello\n", 6) < 0) exit (1); close (fd); } { struct stat statbuf; if (stat ("t-bin-out0.tmp", &statbuf) < 0) exit (1); ASSERT (statbuf.st_size == 6); } switch (argv[1][0]) { case '1': /* Test the set_binary_mode() function. */ set_binary_mode (1, O_BINARY); fputs ("Hello\n", stdout); break; default: break; } return 0; } gnuastro-0.5/bootstrapped/tests/test-arpa_inet.c0000644000175000017500000000156413217200023017070 00000000000000/* Test of substitute. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include int main (void) { return 0; } gnuastro-0.5/bootstrapped/tests/test-argp.c0000644000175000017500000002427413217200023016062 00000000000000/* Test suite for argp. Copyright (C) 2006-2007, 2009-2017 Free Software Foundation, Inc. This file is part of the GNUlib Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "argp.h" #include #include #include #if HAVE_STRINGS_H # include #endif #include "macros.h" struct test_args { int test; int verbose; char *file; int read; char *hidden; int opt; char *optional; int optional_set; int group_2_1_option; int group_1_1_option; }; static struct argp_option group1_option[] = { { NULL, 0, NULL, 0, "Option Group 1", 0 }, { "verbose", 'v', NULL, 0, "Simple option without arguments", 1 }, { "file", 'f', "FILE", 0, "Option with a mandatory argument", 1 }, { "input", 0, NULL, OPTION_ALIAS, NULL, 1 }, { "read", 'r', NULL, OPTION_ALIAS, NULL, 1 }, { "hidden", 'H', "FILE", OPTION_HIDDEN, "Hidden option", 1 }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group1_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'v': args->verbose++; break; case 'r': args->read = 1; FALLTHROUGH; case 'f': args->file = arg; break; case 'H': args->hidden = arg; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group1_argp = { group1_option, group1_parser }; struct argp_child group1_child = { &group1_argp, 0, "", 1 }; static struct argp_option group1_1_option[] = { { NULL, 0, NULL, 0, "Option Group 1.1", 0 }, { "cantiga", 'C', NULL, 0, "create a cantiga" }, { "sonet", 'S', NULL, 0, "create a sonet" }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group1_1_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'C': case 'S': args->group_1_1_option = key; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group1_1_argp = { group1_1_option, group1_1_parser }; struct argp_child group1_1_child = { &group1_1_argp, 0, "", 2 }; static struct argp_option group2_option[] = { { NULL, 0, NULL, 0, "Option Group 2", 0 }, { "option", 'O', NULL, 0, "An option", 1 }, { "optional", 'o', "ARG", OPTION_ARG_OPTIONAL, "Option with an optional argument. ARG is one of the following:", 2 }, { "one", 0, NULL, OPTION_DOC | OPTION_NO_TRANS, "one unit", 3 }, { "two", 0, NULL, OPTION_DOC | OPTION_NO_TRANS, "two units", 3 }, { "many", 0, NULL, OPTION_DOC | OPTION_NO_TRANS, "many units", 3 }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group2_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'O': args->opt = 1; break; case 'o': args->optional_set = 1; args->optional = arg; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group2_argp = { group2_option, group2_parser }; struct argp_child group2_child = { &group2_argp, 0, "", 2 }; static struct argp_option group2_1_option[] = { { NULL, 0, NULL, 0, "Option Group 2.1", 0 }, { "poem", 'p', NULL, 0, "create a poem" }, { "limerick", 'l', NULL, 0, "create a limerick" }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t group2_1_parser (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; switch (key) { case 'p': case 'e': args->group_2_1_option = key; break; default: return ARGP_ERR_UNKNOWN; } return 0; } struct argp group2_1_argp = { group2_1_option, group2_1_parser }; struct argp_child group2_1_child = { &group2_1_argp, 0, "", 2 }; static struct argp_option main_options[] = { { NULL, 0, NULL, 0, "Main options", 0 }, { "test", 't', NULL, 0, NULL, 1 }, { NULL, 0, NULL, 0, NULL, 0 } }; static error_t parse_opt (int key, char *arg, struct argp_state *state) { struct test_args *args = state->input; int i; switch (key) { case ARGP_KEY_INIT: for (i = 0; state->root_argp->children[i].argp; i++) state->child_inputs[i] = args; break; case 't': args->test = 1; break; default: return ARGP_ERR_UNKNOWN; } return 0; } const char *argp_program_version = "test_argp (" PACKAGE_NAME ") " VERSION; const char *argp_program_bug_address = "<" PACKAGE_BUGREPORT ">"; static char doc[] = "documentation string"; struct argp test_argp = { main_options, parse_opt, "ARGS...", doc, NULL, NULL, NULL }; #define NARGS(a) (sizeof(a) / sizeof((a)[0]) - 1) #define ARGV0 "test-argp" #define init_args(a) memset (&(a), 0, sizeof (a)); #define INIT_TEST_COMMON(n) \ int argc = NARGS (argv); \ struct test_args test_args; \ init_args (test_args); \ test_number = n; #define INIT_TEST1(n, arg1) \ char *argv[] = { ARGV0, arg1, NULL }; \ INIT_TEST_COMMON (n) #define INIT_TEST2(n, arg1, arg2) \ char *argv[] = { ARGV0, arg1, arg2, NULL }; \ INIT_TEST_COMMON (n) #define INIT_TEST3(n, arg1, arg2, arg3) \ char *argv[] = { ARGV0, arg1, arg2, arg3, NULL }; \ INIT_TEST_COMMON (n) int test_number; unsigned failure_count = 0; void fail (const char *msg) { fprintf (stderr, "Test %d: %s\n", test_number, msg); failure_count++; } void test1 (struct argp *argp) { INIT_TEST1 (1, "--test"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.test != 1) fail ("option not processed"); } void test2 (struct argp *argp) { INIT_TEST1 (2, "-t"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.test != 1) fail ("option not processed"); } void test_file (struct argp *argp, int argc, char **argv, struct test_args *args) { if (argp_parse (argp, argc, argv, 0, NULL, args)) fail ("argp_parse failed"); else if (!args->file) fail ("option not processed"); else if (strcmp (args->file, "FILE")) fail ("option processed incorrectly"); } void test3 (struct argp *argp) { INIT_TEST1 (3, "--file=FILE"); test_file (argp, argc, argv, &test_args); } void test4 (struct argp *argp) { INIT_TEST2 (4, "--file", "FILE"); test_file (argp, argc, argv, &test_args); } void test5 (struct argp *argp) { INIT_TEST1 (5, "--input=FILE"); test_file (argp, argc, argv, &test_args); } void test6 (struct argp *argp) { INIT_TEST2 (6, "--input", "FILE"); test_file (argp, argc, argv, &test_args); } void test_optional (struct argp *argp, int argc, char **argv, struct test_args *args, const char *val, const char *a) { int index; if (argp_parse (argp, argc, argv, 0, &index, args)) fail ("argp_parse failed"); else if (!args->optional_set) fail ("option not processed"); if (!val) { if (args->optional) fail ("option processed incorrectly"); } else if (strcmp (args->optional, val)) fail ("option processed incorrectly"); if (a) { if (index == argc) fail ("expected command line argument not found"); else if (strcmp (argv[index], a)) fail ("expected command line argument does not match"); } } void test7 (struct argp *argp) { INIT_TEST1 (7, "-oARG"); test_optional (argp, argc, argv, &test_args, "ARG", NULL); } void test8 (struct argp *argp) { INIT_TEST2 (8, "-o", "ARG"); test_optional (argp, argc, argv, &test_args, NULL, "ARG"); } void test9 (struct argp *argp) { INIT_TEST1 (9, "--optional=ARG"); test_optional (argp, argc, argv, &test_args, "ARG", NULL); } void test10 (struct argp *argp) { INIT_TEST2 (10, "--optional", "ARG"); test_optional (argp, argc, argv, &test_args, NULL, "ARG"); } void test11 (struct argp *argp) { INIT_TEST1 (11, "--optiona=ARG"); test_optional (argp, argc, argv, &test_args, "ARG", NULL); } void test12 (struct argp *argp) { INIT_TEST3 (12, "--option", "--optional=OPT", "FILE"); test_optional (argp, argc, argv, &test_args, "OPT", "FILE"); } void test13 (struct argp *argp) { INIT_TEST1 (1, "--cantiga"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.group_1_1_option != 'C') fail ("option not processed"); } void test14 (struct argp *argp) { INIT_TEST1 (1, "--limerick"); if (argp_parse (argp, argc, argv, 0, NULL, &test_args)) fail ("argp_parse failed"); else if (test_args.group_2_1_option != 'l') fail ("option not processed"); } void test15 (struct argp *argp) { INIT_TEST2 (1, "-r", "FILE"); test_file (argp, argc, argv, &test_args); if (!test_args.read) fail ("short alias not recognized properly"); } typedef void (*test_fp) (struct argp *argp); test_fp test_fun[] = { test1, test2, test3, test4, test5, test6, test7, test8, test9, test10, test11, test12, test13, test14, test15, NULL }; int main (int argc, char **argv) { struct argp_child argp_children[3], group1_children[2], group2_children[2]; test_fp *fun; group1_children[0] = group1_1_child; group1_children[1].argp = NULL; group1_argp.children = group1_children; group2_children[0] = group2_1_child; group2_children[1].argp = NULL; group2_argp.children = group2_children; argp_children[0] = group1_child; argp_children[1] = group2_child; argp_children[2].argp = NULL; test_argp.children = argp_children; if (argc > 0) { struct test_args test_args; init_args (test_args); return argp_parse (&test_argp, argc, argv, 0, NULL, &test_args); } for (fun = test_fun; *fun; fun++) (*fun) (&test_argp); if (failure_count) return 1; return 0; } gnuastro-0.5/bootstrapped/tests/test-alloca-opt.c0000644000175000017500000000276313217200023017163 00000000000000/* Test of optional automatic memory allocation. Copyright (C) 2005, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include #if HAVE_ALLOCA static void do_allocation (int n) { void *ptr = alloca (n); (void) ptr; } void (*func) (int) = do_allocation; #endif int main () { #if HAVE_ALLOCA int i; /* Repeat a lot of times, to make sure there's no memory leak. */ for (i = 0; i < 100000; i++) { /* Try various values. n = 0 gave a crash on Alpha with gcc-2.5.8. Some versions of Mac OS X have a stack size limit of 512 KB. */ func (34); func (134); func (399); func (510823); func (129321); func (0); func (4070); func (4095); func (1); func (16582); } #endif return 0; } gnuastro-0.5/bootstrapped/tests/test-accept.c0000644000175000017500000000277313217200023016370 00000000000000/* Test accepting a connection to a server socket. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include "signature.h" SIGNATURE_CHECK (accept, int, (int, struct sockaddr *, socklen_t *)); #include #include #include #include "sockets.h" #include "macros.h" int main (void) { (void) gl_sockets_startup (SOCKETS_1_1); /* Test behaviour for invalid file descriptors. */ { struct sockaddr_in addr; socklen_t addrlen = sizeof (addr); errno = 0; ASSERT (accept (-1, (struct sockaddr *) &addr, &addrlen) == -1); ASSERT (errno == EBADF); } { struct sockaddr_in addr; socklen_t addrlen = sizeof (addr); close (99); errno = 0; ASSERT (accept (99, (struct sockaddr *) &addr, &addrlen) == -1); ASSERT (errno == EBADF); } return 0; } gnuastro-0.5/bootstrapped/tests/wctomb.c0000644000175000017500000000162413217200024015442 00000000000000/* Convert wide character to multibyte character. Copyright (C) 2011-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include "wctomb-impl.h" gnuastro-0.5/bootstrapped/tests/wctob.c0000644000175000017500000000226513217200024015267 00000000000000/* Convert wide character to unibyte character. Copyright (C) 2008, 2010-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include int wctob (wint_t wc) { char buf[64]; if (!(MB_CUR_MAX <= sizeof (buf))) abort (); /* Handle the case where WEOF is a value that does not fit in a wchar_t. */ if (wc == (wchar_t)wc) if (wctomb (buf, (wchar_t)wc) == 1) return (unsigned char) buf[0]; return EOF; } gnuastro-0.5/bootstrapped/tests/usleep.c0000644000175000017500000000350313217200024015442 00000000000000/* Pausing execution of the current thread. Copyright (C) 2009-2017 Free Software Foundation, Inc. Written by Eric Blake , 2009. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This file is _intentionally_ light-weight. Rather than using select or nanosleep, both of which drag in external libraries on some platforms, this merely rounds up to the nearest second if usleep() does not exist. If sub-second resolution is important, then use a more powerful interface to begin with. */ #include /* Specification. */ #include #include #ifndef HAVE_USLEEP # define HAVE_USLEEP 0 #endif /* Sleep for MICRO microseconds, which can be greater than 1 second. Return -1 and set errno to EINVAL on range error (about 4295 seconds), or 0 on success. Interaction with SIGALARM is unspecified. */ int usleep (useconds_t micro) { unsigned int seconds = micro / 1000000; if (sizeof seconds < sizeof micro && micro / 1000000 != seconds) { errno = EINVAL; return -1; } if (!HAVE_USLEEP && micro % 1000000) seconds++; while ((seconds = sleep (seconds)) != 0); #undef usleep #if !HAVE_USLEEP # define usleep(x) 0 #endif return usleep (micro % 1000000); } gnuastro-0.5/bootstrapped/tests/unsetenv.c0000644000175000017500000000547313217200024016024 00000000000000/* Copyright (C) 1992, 1995-2002, 2005-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Don't use __attribute__ __nonnull__ in this compilation unit. Otherwise gcc optimizes away the name == NULL test below. */ #define _GL_ARG_NONNULL(params) #include /* Specification. */ #include #include #if !_LIBC # define __set_errno(ev) ((errno) = (ev)) #endif #include #include #if !_LIBC # define __environ environ #endif #if _LIBC /* This lock protects against simultaneous modifications of 'environ'. */ # include __libc_lock_define_initialized (static, envlock) # define LOCK __libc_lock_lock (envlock) # define UNLOCK __libc_lock_unlock (envlock) #else # define LOCK # define UNLOCK #endif /* In the GNU C library we must keep the namespace clean. */ #ifdef _LIBC # define unsetenv __unsetenv #endif #if _LIBC || !HAVE_UNSETENV int unsetenv (const char *name) { size_t len; char **ep; if (name == NULL || *name == '\0' || strchr (name, '=') != NULL) { __set_errno (EINVAL); return -1; } len = strlen (name); LOCK; ep = __environ; while (*ep != NULL) if (!strncmp (*ep, name, len) && (*ep)[len] == '=') { /* Found it. Remove this pointer by moving later ones back. */ char **dp = ep; do dp[0] = dp[1]; while (*dp++); /* Continue the loop in case NAME appears again. */ } else ++ep; UNLOCK; return 0; } #ifdef _LIBC # undef unsetenv weak_alias (__unsetenv, unsetenv) #endif #else /* HAVE_UNSETENV */ # undef unsetenv # if !HAVE_DECL_UNSETENV # if VOID_UNSETENV extern void unsetenv (const char *); # else extern int unsetenv (const char *); # endif # endif /* Call the underlying unsetenv, in case there is hidden bookkeeping that needs updating beyond just modifying environ. */ int rpl_unsetenv (const char *name) { int result = 0; if (!name || !*name || strchr (name, '=')) { errno = EINVAL; return -1; } while (getenv (name)) # if !VOID_UNSETENV result = # endif unsetenv (name); return result; } #endif /* HAVE_UNSETENV */ gnuastro-0.5/bootstrapped/tests/symlink.c0000644000175000017500000000263213217200023015634 00000000000000/* Stub for symlink(). Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include #if HAVE_SYMLINK # undef symlink /* Create a symlink, but reject trailing slash. */ int rpl_symlink (char const *contents, char const *name) { size_t len = strlen (name); if (len && name[len - 1] == '/') { struct stat st; if (lstat (name, &st) == 0) errno = EEXIST; return -1; } return symlink (contents, name); } #else /* !HAVE_SYMLINK */ /* The system does not support symlinks. */ int symlink (char const *contents _GL_UNUSED, char const *name _GL_UNUSED) { errno = ENOSYS; return -1; } #endif /* !HAVE_SYMLINK */ gnuastro-0.5/bootstrapped/tests/strerror_r.c0000644000175000017500000003261113217200023016351 00000000000000/* strerror_r.c --- POSIX compatible system error routine Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2010. */ #include /* Enable declaration of sys_nerr and sys_errlist in on NetBSD. */ #define _NETBSD_SOURCE 1 /* Specification. */ #include #include #include #include #if !HAVE_SNPRINTF # include #endif #include "strerror-override.h" #if (__GLIBC__ >= 2 || defined __UCLIBC__ || defined __CYGWIN__) && HAVE___XPG_STRERROR_R /* glibc >= 2.3.4, cygwin >= 1.7.9 */ # define USE_XPG_STRERROR_R 1 extern #ifdef __cplusplus "C" #endif int __xpg_strerror_r (int errnum, char *buf, size_t buflen); #elif HAVE_DECL_STRERROR_R && !(__GLIBC__ >= 2 || defined __UCLIBC__ || defined __CYGWIN__) /* The system's strerror_r function is OK, except that its third argument is 'int', not 'size_t', or its return type is wrong. */ # include # define USE_SYSTEM_STRERROR_R 1 #else /* (__GLIBC__ >= 2 || defined __UCLIBC__ || defined __CYGWIN__ ? !HAVE___XPG_STRERROR_R : !HAVE_DECL_STRERROR_R) */ /* Use the system's strerror(). Exclude glibc and cygwin because the system strerror_r has the wrong return type, and cygwin 1.7.9 strerror_r clobbers strerror. */ # undef strerror # define USE_SYSTEM_STRERROR 1 # if defined __NetBSD__ || defined __hpux || ((defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__) || defined __sgi || (defined __sun && !defined _LP64) || defined __CYGWIN__ /* No locking needed. */ /* Get catgets internationalization functions. */ # if HAVE_CATGETS # include # endif #ifdef __cplusplus extern "C" { #endif /* Get sys_nerr, sys_errlist on HP-UX (otherwise only declared in C++ mode). Get sys_nerr, sys_errlist on IRIX (otherwise only declared with _SGIAPI). */ # if defined __hpux || defined __sgi extern int sys_nerr; extern char *sys_errlist[]; # endif /* Get sys_nerr on Solaris. */ # if defined __sun && !defined _LP64 extern int sys_nerr; # endif #ifdef __cplusplus } #endif # else # include "glthread/lock.h" /* This lock protects the buffer returned by strerror(). We assume that no other uses of strerror() exist in the program. */ gl_lock_define_initialized(static, strerror_lock) # endif #endif /* On MSVC, there is no snprintf() function, just a _snprintf(). It is of lower quality, but sufficient for the simple use here. We only have to make sure to NUL terminate the result (_snprintf does not NUL terminate, like strncpy). */ #if !HAVE_SNPRINTF static int local_snprintf (char *buf, size_t buflen, const char *format, ...) { va_list args; int result; va_start (args, format); result = _vsnprintf (buf, buflen, format, args); va_end (args); if (buflen > 0 && (result < 0 || result >= buflen)) buf[buflen - 1] = '\0'; return result; } # define snprintf local_snprintf #endif /* Copy as much of MSG into BUF as possible, without corrupting errno. Return 0 if MSG fit in BUFLEN, otherwise return ERANGE. */ static int safe_copy (char *buf, size_t buflen, const char *msg) { size_t len = strlen (msg); int ret; if (len < buflen) { /* Although POSIX allows memcpy() to corrupt errno, we don't know of any implementation where this is a real problem. */ memcpy (buf, msg, len + 1); ret = 0; } else { memcpy (buf, msg, buflen - 1); buf[buflen - 1] = '\0'; ret = ERANGE; } return ret; } int strerror_r (int errnum, char *buf, size_t buflen) #undef strerror_r { /* Filter this out now, so that rest of this replacement knows that there is room for a non-empty message and trailing NUL. */ if (buflen <= 1) { if (buflen) *buf = '\0'; return ERANGE; } *buf = '\0'; /* Check for gnulib overrides. */ { char const *msg = strerror_override (errnum); if (msg) return safe_copy (buf, buflen, msg); } { int ret; int saved_errno = errno; #if USE_XPG_STRERROR_R { ret = __xpg_strerror_r (errnum, buf, buflen); if (ret < 0) ret = errno; if (!*buf) { /* glibc 2.13 would not touch buf on err, so we have to fall back to GNU strerror_r which always returns a thread-safe untruncated string to (partially) copy into our buf. */ safe_copy (buf, buflen, strerror_r (errnum, buf, buflen)); } } #elif USE_SYSTEM_STRERROR_R if (buflen > INT_MAX) buflen = INT_MAX; # ifdef __hpux /* On HP-UX 11.31, strerror_r always fails when buflen < 80; it also fails to change buf on EINVAL. */ { char stackbuf[80]; if (buflen < sizeof stackbuf) { ret = strerror_r (errnum, stackbuf, sizeof stackbuf); if (ret == 0) ret = safe_copy (buf, buflen, stackbuf); } else ret = strerror_r (errnum, buf, buflen); } # else ret = strerror_r (errnum, buf, buflen); /* Some old implementations may return (-1, EINVAL) instead of EINVAL. But on Haiku, valid error numbers are negative. */ # if !defined __HAIKU__ if (ret < 0) ret = errno; # endif # endif # if defined _AIX || defined __HAIKU__ /* AIX and Haiku return 0 rather than ERANGE when truncating strings; try again until we are sure we got the entire string. */ if (!ret && strlen (buf) == buflen - 1) { char stackbuf[STACKBUF_LEN]; size_t len; strerror_r (errnum, stackbuf, sizeof stackbuf); len = strlen (stackbuf); /* STACKBUF_LEN should have been large enough. */ if (len + 1 == sizeof stackbuf) abort (); if (buflen <= len) ret = ERANGE; } # else /* Solaris 10 does not populate buf on ERANGE. OpenBSD 4.7 truncates early on ERANGE rather than return a partial integer. We prefer the maximal string. We set buf[0] earlier, and we know of no implementation that modifies buf to be an unterminated string, so this strlen should be portable in practice (rather than pulling in a safer strnlen). */ if (ret == ERANGE && strlen (buf) < buflen - 1) { char stackbuf[STACKBUF_LEN]; /* STACKBUF_LEN should have been large enough. */ if (strerror_r (errnum, stackbuf, sizeof stackbuf) == ERANGE) abort (); safe_copy (buf, buflen, stackbuf); } # endif #else /* USE_SYSTEM_STRERROR */ /* Try to do what strerror (errnum) does, but without clobbering the buffer used by strerror(). */ # if defined __NetBSD__ || defined __hpux || ((defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__) || defined __CYGWIN__ /* NetBSD, HP-UX, native Windows, Cygwin */ /* NetBSD: sys_nerr, sys_errlist are declared through _NETBSD_SOURCE and above. HP-UX: sys_nerr, sys_errlist are declared explicitly above. native Windows: sys_nerr, sys_errlist are declared in . Cygwin: sys_nerr, sys_errlist are declared in . */ if (errnum >= 0 && errnum < sys_nerr) { # if HAVE_CATGETS && (defined __NetBSD__ || defined __hpux) # if defined __NetBSD__ nl_catd catd = catopen ("libc", NL_CAT_LOCALE); const char *errmsg = (catd != (nl_catd)-1 ? catgets (catd, 1, errnum, sys_errlist[errnum]) : sys_errlist[errnum]); # endif # if defined __hpux nl_catd catd = catopen ("perror", NL_CAT_LOCALE); const char *errmsg = (catd != (nl_catd)-1 ? catgets (catd, 1, 1 + errnum, sys_errlist[errnum]) : sys_errlist[errnum]); # endif # else const char *errmsg = sys_errlist[errnum]; # endif if (errmsg == NULL || *errmsg == '\0') ret = EINVAL; else ret = safe_copy (buf, buflen, errmsg); # if HAVE_CATGETS && (defined __NetBSD__ || defined __hpux) if (catd != (nl_catd)-1) catclose (catd); # endif } else ret = EINVAL; # elif defined __sgi || (defined __sun && !defined _LP64) /* IRIX, Solaris <= 9 32-bit */ /* For a valid error number, the system's strerror() function returns a pointer to a not copied string, not to a buffer. */ if (errnum >= 0 && errnum < sys_nerr) { char *errmsg = strerror (errnum); if (errmsg == NULL || *errmsg == '\0') ret = EINVAL; else ret = safe_copy (buf, buflen, errmsg); } else ret = EINVAL; # else gl_lock_lock (strerror_lock); { char *errmsg = strerror (errnum); /* For invalid error numbers, strerror() on - IRIX 6.5 returns NULL, - HP-UX 11 returns an empty string. */ if (errmsg == NULL || *errmsg == '\0') ret = EINVAL; else ret = safe_copy (buf, buflen, errmsg); } gl_lock_unlock (strerror_lock); # endif #endif #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* MSVC 14 defines names for many error codes in the range 100..140, but _sys_errlist contains strings only for the error codes < _sys_nerr = 43. */ if (ret == EINVAL) { const char *errmsg; switch (errnum) { case 100 /* EADDRINUSE */: errmsg = "Address already in use"; break; case 101 /* EADDRNOTAVAIL */: errmsg = "Cannot assign requested address"; break; case 102 /* EAFNOSUPPORT */: errmsg = "Address family not supported by protocol"; break; case 103 /* EALREADY */: errmsg = "Operation already in progress"; break; case 105 /* ECANCELED */: errmsg = "Operation canceled"; break; case 106 /* ECONNABORTED */: errmsg = "Software caused connection abort"; break; case 107 /* ECONNREFUSED */: errmsg = "Connection refused"; break; case 108 /* ECONNRESET */: errmsg = "Connection reset by peer"; break; case 109 /* EDESTADDRREQ */: errmsg = "Destination address required"; break; case 110 /* EHOSTUNREACH */: errmsg = "No route to host"; break; case 112 /* EINPROGRESS */: errmsg = "Operation now in progress"; break; case 113 /* EISCONN */: errmsg = "Transport endpoint is already connected"; break; case 114 /* ELOOP */: errmsg = "Too many levels of symbolic links"; break; case 115 /* EMSGSIZE */: errmsg = "Message too long"; break; case 116 /* ENETDOWN */: errmsg = "Network is down"; break; case 117 /* ENETRESET */: errmsg = "Network dropped connection on reset"; break; case 118 /* ENETUNREACH */: errmsg = "Network is unreachable"; break; case 119 /* ENOBUFS */: errmsg = "No buffer space available"; break; case 123 /* ENOPROTOOPT */: errmsg = "Protocol not available"; break; case 126 /* ENOTCONN */: errmsg = "Transport endpoint is not connected"; break; case 128 /* ENOTSOCK */: errmsg = "Socket operation on non-socket"; break; case 129 /* ENOTSUP */: errmsg = "Not supported"; break; case 130 /* EOPNOTSUPP */: errmsg = "Operation not supported"; break; case 132 /* EOVERFLOW */: errmsg = "Value too large for defined data type"; break; case 133 /* EOWNERDEAD */: errmsg = "Owner died"; break; case 134 /* EPROTO */: errmsg = "Protocol error"; break; case 135 /* EPROTONOSUPPORT */: errmsg = "Protocol not supported"; break; case 136 /* EPROTOTYPE */: errmsg = "Protocol wrong type for socket"; break; case 138 /* ETIMEDOUT */: errmsg = "Connection timed out"; break; case 140 /* EWOULDBLOCK */: errmsg = "Operation would block"; break; default: errmsg = NULL; break; } if (errmsg != NULL) ret = safe_copy (buf, buflen, errmsg); } #endif if (ret == EINVAL && !*buf) { #if defined __HAIKU__ /* For consistency with perror(). */ snprintf (buf, buflen, "Unknown Application Error (%d)", errnum); #else snprintf (buf, buflen, "Unknown error %d", errnum); #endif } errno = saved_errno; return ret; } } gnuastro-0.5/bootstrapped/tests/stat.c0000644000175000017500000003174013217200023015123 00000000000000/* Work around platform bugs in stat. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake and Bruno Haible. */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_stat doesn't recurse to rpl_stat. */ #define __need_system_sys_stat_h #include /* Get the original definition of stat. It might be defined as a macro. */ #include #include #undef __need_system_sys_stat_h #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WINDOWS_NATIVE #endif #if !defined WINDOWS_NATIVE static int orig_stat (const char *filename, struct stat *buf) { return stat (filename, buf); } #endif /* Specification. */ /* Write "sys/stat.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ #include "sys/stat.h" #include "stat-time.h" #include #include #include #include #include "filename.h" #include "malloca.h" #include "verify.h" #ifdef WINDOWS_NATIVE # define WIN32_LEAN_AND_MEAN # include # include "stat-w32.h" #endif #ifdef WINDOWS_NATIVE /* Return TRUE if the given file name denotes an UNC root. */ static BOOL is_unc_root (const char *rname) { /* Test whether it has the syntax '\\server\share'. */ if (ISSLASH (rname[0]) && ISSLASH (rname[1])) { /* It starts with two slashes. Find the next slash. */ const char *p = rname + 2; const char *q = p; while (*q != '\0' && !ISSLASH (*q)) q++; if (q > p && *q != '\0') { /* Found the next slash at q. */ q++; const char *r = q; while (*r != '\0' && !ISSLASH (*r)) r++; if (r > q && *r == '\0') return TRUE; } } return FALSE; } #endif /* Store information about NAME into ST. Work around bugs with trailing slashes. Mingw has other bugs (such as st_ino always being 0 on success) which this wrapper does not work around. But at least this implementation provides the ability to emulate fchdir correctly. */ int rpl_stat (char const *name, struct stat *buf) { #ifdef WINDOWS_NATIVE /* Fill the fields ourselves, because the original stat function returns values for st_atime, st_mtime, st_ctime that depend on the current time zone. See */ /* XXX Should we convert to wchar_t* and prepend '\\?\', in order to work around length limitations ? */ /* POSIX specifies: "More than two leading characters shall be treated as a single character." */ if (ISSLASH (name[0]) && ISSLASH (name[1]) && ISSLASH (name[2])) { name += 2; while (ISSLASH (name[1])) name++; } size_t len = strlen (name); size_t drive_prefix_len = (HAS_DEVICE (name) ? 2 : 0); /* Remove trailing slashes (except the very first one, at position drive_prefix_len), but remember their presence. */ size_t rlen; bool check_dir = false; rlen = len; while (rlen > drive_prefix_len && ISSLASH (name[rlen-1])) { check_dir = true; if (rlen == drive_prefix_len + 1) break; rlen--; } /* Handle '' and 'C:'. */ if (!check_dir && rlen == drive_prefix_len) { errno = ENOENT; return -1; } /* Handle '\\'. */ if (rlen == 1 && ISSLASH (name[0]) && len >= 2) { errno = ENOENT; return -1; } const char *rname; char *malloca_rname; if (rlen == len) { rname = name; malloca_rname = NULL; } else { malloca_rname = malloca (rlen + 1); if (malloca_rname == NULL) { errno = ENOMEM; return -1; } memcpy (malloca_rname, name, rlen); malloca_rname[rlen] = '\0'; rname = malloca_rname; } /* There are two ways to get at the requested information: - by scanning the parent directory and examining the relevant directory entry, - by opening the file directly. The first approach fails for root directories (e.g. 'C:\') and UNC root directories (e.g. '\\server\share'). The second approach fails for some system files (e.g. 'C:\pagefile.sys' and 'C:\hiberfil.sys'): ERROR_SHARING_VIOLATION. The second approach gives more information (in particular, correct st_dev, st_ino, st_nlink fields). So we use the second approach and, as a fallback except for root and UNC root directories, also the first approach. */ { int ret; { /* Approach based on the file. */ /* Open a handle to the file. CreateFile */ HANDLE h = CreateFile (rname, FILE_READ_ATTRIBUTES, FILE_SHARE_READ | FILE_SHARE_WRITE | FILE_SHARE_DELETE, NULL, OPEN_EXISTING, /* FILE_FLAG_POSIX_SEMANTICS (treat file names that differ only in case as different) makes sense only when applied to *all* filesystem operations. */ FILE_FLAG_BACKUP_SEMANTICS /* | FILE_FLAG_POSIX_SEMANTICS */, NULL); if (h != INVALID_HANDLE_VALUE) { ret = _gl_fstat_by_handle (h, rname, buf); CloseHandle (h); goto done; } } /* Test for root and UNC root directories. */ if ((rlen == drive_prefix_len + 1 && ISSLASH (rname[drive_prefix_len])) || is_unc_root (rname)) goto failed; /* Fallback. */ { /* Approach based on the directory entry. */ if (strchr (rname, '?') != NULL || strchr (rname, '*') != NULL) { /* Other Windows API functions would fail with error ERROR_INVALID_NAME. */ if (malloca_rname != NULL) freea (malloca_rname); errno = ENOENT; return -1; } /* Get the details about the directory entry. This can be done through FindFirstFile or through FindFirstFileEx with argument FindExInfoBasic */ WIN32_FIND_DATA info; HANDLE h = FindFirstFile (rname, &info); if (h == INVALID_HANDLE_VALUE) goto failed; /* Test for error conditions before starting to fill *buf. */ if (sizeof (buf->st_size) <= 4 && info.nFileSizeHigh > 0) { FindClose (h); if (malloca_rname != NULL) freea (malloca_rname); errno = EOVERFLOW; return -1; } # if _GL_WINDOWS_STAT_INODES buf->st_dev = 0; # if _GL_WINDOWS_STAT_INODES == 2 buf->st_ino._gl_ino[0] = buf->st_ino._gl_ino[1] = 0; # else /* _GL_WINDOWS_STAT_INODES == 1 */ buf->st_ino = 0; # endif # else /* st_ino is not wide enough for identifying a file on a device. Without st_ino, st_dev is pointless. */ buf->st_dev = 0; buf->st_ino = 0; # endif /* st_mode. */ unsigned int mode = /* XXX How to handle FILE_ATTRIBUTE_REPARSE_POINT ? */ ((info.dwFileAttributes & FILE_ATTRIBUTE_DIRECTORY) ? _S_IFDIR | S_IEXEC_UGO : _S_IFREG) | S_IREAD_UGO | ((info.dwFileAttributes & FILE_ATTRIBUTE_READONLY) ? 0 : S_IWRITE_UGO); if (!(info.dwFileAttributes & FILE_ATTRIBUTE_DIRECTORY)) { /* Determine whether the file is executable by looking at the file name suffix. */ if (info.nFileSizeHigh > 0 || info.nFileSizeLow > 0) { const char *last_dot = NULL; const char *p; for (p = info.cFileName; *p != '\0'; p++) if (*p == '.') last_dot = p; if (last_dot != NULL) { const char *suffix = last_dot + 1; if (_stricmp (suffix, "exe") == 0 || _stricmp (suffix, "bat") == 0 || _stricmp (suffix, "cmd") == 0 || _stricmp (suffix, "com") == 0) mode |= S_IEXEC_UGO; } } } buf->st_mode = mode; /* st_nlink. Ignore hard links here. */ buf->st_nlink = 1; /* There's no easy way to map the Windows SID concept to an integer. */ buf->st_uid = 0; buf->st_gid = 0; /* st_rdev is irrelevant for normal files and directories. */ buf->st_rdev = 0; /* st_size. */ if (sizeof (buf->st_size) <= 4) /* Range check already done above. */ buf->st_size = info.nFileSizeLow; else buf->st_size = ((long long) info.nFileSizeHigh << 32) | (long long) info.nFileSizeLow; /* st_atime, st_mtime, st_ctime. */ # if _GL_WINDOWS_STAT_TIMESPEC buf->st_atim = _gl_convert_FILETIME_to_timespec (&info.ftLastAccessTime); buf->st_mtim = _gl_convert_FILETIME_to_timespec (&info.ftLastWriteTime); buf->st_ctim = _gl_convert_FILETIME_to_timespec (&info.ftCreationTime); # else buf->st_atime = _gl_convert_FILETIME_to_POSIX (&info.ftLastAccessTime); buf->st_mtime = _gl_convert_FILETIME_to_POSIX (&info.ftLastWriteTime); buf->st_ctime = _gl_convert_FILETIME_to_POSIX (&info.ftCreationTime); # endif FindClose (h); ret = 0; } done: if (ret >= 0 && check_dir && !S_ISDIR (buf->st_mode)) { errno = ENOTDIR; ret = -1; } if (malloca_rname != NULL) { int saved_errno = errno; freea (malloca_rname); errno = saved_errno; } return ret; } failed: { DWORD error = GetLastError (); #if 0 fprintf (stderr, "rpl_stat error 0x%x\n", (unsigned int) error); #endif if (malloca_rname != NULL) freea (malloca_rname); switch (error) { /* Some of these errors probably cannot happen with the specific flags that we pass to CreateFile. But who knows... */ case ERROR_FILE_NOT_FOUND: /* The last component of rname does not exist. */ case ERROR_PATH_NOT_FOUND: /* Some directory component in rname does not exist. */ case ERROR_BAD_PATHNAME: /* rname is such as '\\server'. */ case ERROR_BAD_NET_NAME: /* rname is such as '\\server\nonexistentshare'. */ case ERROR_INVALID_NAME: /* rname contains wildcards, misplaced colon, etc. */ case ERROR_DIRECTORY: errno = ENOENT; break; case ERROR_ACCESS_DENIED: /* rname is such as 'C:\System Volume Information\foo'. */ case ERROR_SHARING_VIOLATION: /* rname is such as 'C:\pagefile.sys' (second approach only). */ /* XXX map to EACCESS or EPERM? */ errno = EACCES; break; case ERROR_OUTOFMEMORY: errno = ENOMEM; break; case ERROR_WRITE_PROTECT: errno = EROFS; break; case ERROR_WRITE_FAULT: case ERROR_READ_FAULT: case ERROR_GEN_FAILURE: errno = EIO; break; case ERROR_BUFFER_OVERFLOW: case ERROR_FILENAME_EXCED_RANGE: errno = ENAMETOOLONG; break; case ERROR_DELETE_PENDING: /* XXX map to EACCESS or EPERM? */ errno = EPERM; break; default: errno = EINVAL; break; } return -1; } #else int result = orig_stat (name, buf); if (result == 0) { # if REPLACE_FUNC_STAT_FILE /* Solaris 9 mistakenly succeeds when given a non-directory with a trailing slash. */ if (!S_ISDIR (buf->st_mode)) { size_t len = strlen (name); if (ISSLASH (name[len - 1])) { errno = ENOTDIR; return -1; } } # endif /* REPLACE_FUNC_STAT_FILE */ result = stat_time_normalize (result, buf); } return result; #endif } gnuastro-0.5/bootstrapped/tests/socket.c0000644000175000017500000000256513217200023015443 00000000000000/* socket.c --- wrappers for Windows socket function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #define WIN32_LEAN_AND_MEAN /* Get winsock2.h. */ #include /* Get set_winsock_errno, FD_TO_SOCKET etc. */ #include "w32sock.h" #include "sockets.h" int rpl_socket (int domain, int type, int protocol) { SOCKET fh; gl_sockets_startup (SOCKETS_1_1); /* We have to use WSASocket() to create non-overlapped IO sockets. Overlapped IO sockets cannot be used with read/write. */ fh = WSASocket (domain, type, protocol, NULL, 0, 0); if (fh == INVALID_SOCKET) { set_winsock_errno (); return -1; } else return SOCKET_TO_FD (fh); } gnuastro-0.5/bootstrapped/tests/sigprocmask.c0000644000175000017500000002063013217200023016466 00000000000000/* POSIX compatible signal blocking. Copyright (C) 2006-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2006. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif /* We assume that a platform without POSIX signal blocking functions also does not have the POSIX sigaction() function, only the signal() function. We also assume signal() has SysV semantics, where any handler is uninstalled prior to being invoked. This is true for native Windows platforms. */ /* We use raw signal(), but also provide a wrapper rpl_signal() so that applications can query or change a blocked signal. */ #undef signal /* Provide invalid signal numbers as fallbacks if the uncatchable signals are not defined. */ #ifndef SIGKILL # define SIGKILL (-1) #endif #ifndef SIGSTOP # define SIGSTOP (-1) #endif /* On native Windows, as of 2008, the signal SIGABRT_COMPAT is an alias for the signal SIGABRT. Only one signal handler is stored for both SIGABRT and SIGABRT_COMPAT. SIGABRT_COMPAT is not a signal of its own. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # undef SIGABRT_COMPAT # define SIGABRT_COMPAT 6 #endif #ifdef SIGABRT_COMPAT # define SIGABRT_COMPAT_MASK (1U << SIGABRT_COMPAT) #else # define SIGABRT_COMPAT_MASK 0 #endif typedef void (*handler_t) (int); #if HAVE_MSVC_INVALID_PARAMETER_HANDLER static handler_t signal_nothrow (int sig, handler_t handler) { handler_t result; TRY_MSVC_INVAL { result = signal (sig, handler); } CATCH_MSVC_INVAL { result = SIG_ERR; errno = EINVAL; } DONE_MSVC_INVAL; return result; } # define signal signal_nothrow #endif /* Handling of gnulib defined signals. */ #if GNULIB_defined_SIGPIPE static handler_t SIGPIPE_handler = SIG_DFL; #endif #if GNULIB_defined_SIGPIPE static handler_t ext_signal (int sig, handler_t handler) { switch (sig) { case SIGPIPE: { handler_t old_handler = SIGPIPE_handler; SIGPIPE_handler = handler; return old_handler; } default: /* System defined signal */ return signal (sig, handler); } } # undef signal # define signal ext_signal #endif int sigismember (const sigset_t *set, int sig) { if (sig >= 0 && sig < NSIG) { #ifdef SIGABRT_COMPAT if (sig == SIGABRT_COMPAT) sig = SIGABRT; #endif return (*set >> sig) & 1; } else return 0; } int sigemptyset (sigset_t *set) { *set = 0; return 0; } int sigaddset (sigset_t *set, int sig) { if (sig >= 0 && sig < NSIG) { #ifdef SIGABRT_COMPAT if (sig == SIGABRT_COMPAT) sig = SIGABRT; #endif *set |= 1U << sig; return 0; } else { errno = EINVAL; return -1; } } int sigdelset (sigset_t *set, int sig) { if (sig >= 0 && sig < NSIG) { #ifdef SIGABRT_COMPAT if (sig == SIGABRT_COMPAT) sig = SIGABRT; #endif *set &= ~(1U << sig); return 0; } else { errno = EINVAL; return -1; } } int sigfillset (sigset_t *set) { *set = ((2U << (NSIG - 1)) - 1) & ~ SIGABRT_COMPAT_MASK; return 0; } /* Set of currently blocked signals. */ static volatile sigset_t blocked_set /* = 0 */; /* Set of currently blocked and pending signals. */ static volatile sig_atomic_t pending_array[NSIG] /* = { 0 } */; /* Signal handler that is installed for blocked signals. */ static void blocked_handler (int sig) { /* Reinstall the handler, in case the signal occurs multiple times while blocked. There is an inherent race where an asynchronous signal in between when the kernel uninstalled the handler and when we reinstall it will trigger the default handler; oh well. */ signal (sig, blocked_handler); if (sig >= 0 && sig < NSIG) pending_array[sig] = 1; } int sigpending (sigset_t *set) { sigset_t pending = 0; int sig; for (sig = 0; sig < NSIG; sig++) if (pending_array[sig]) pending |= 1U << sig; *set = pending; return 0; } /* The previous signal handlers. Only the array elements corresponding to blocked signals are relevant. */ static volatile handler_t old_handlers[NSIG]; int sigprocmask (int operation, const sigset_t *set, sigset_t *old_set) { if (old_set != NULL) *old_set = blocked_set; if (set != NULL) { sigset_t new_blocked_set; sigset_t to_unblock; sigset_t to_block; switch (operation) { case SIG_BLOCK: new_blocked_set = blocked_set | *set; break; case SIG_SETMASK: new_blocked_set = *set; break; case SIG_UNBLOCK: new_blocked_set = blocked_set & ~*set; break; default: errno = EINVAL; return -1; } to_unblock = blocked_set & ~new_blocked_set; to_block = new_blocked_set & ~blocked_set; if (to_block != 0) { int sig; for (sig = 0; sig < NSIG; sig++) if ((to_block >> sig) & 1) { pending_array[sig] = 0; if ((old_handlers[sig] = signal (sig, blocked_handler)) != SIG_ERR) blocked_set |= 1U << sig; } } if (to_unblock != 0) { sig_atomic_t received[NSIG]; int sig; for (sig = 0; sig < NSIG; sig++) if ((to_unblock >> sig) & 1) { if (signal (sig, old_handlers[sig]) != blocked_handler) /* The application changed a signal handler while the signal was blocked, bypassing our rpl_signal replacement. We don't support this. */ abort (); received[sig] = pending_array[sig]; blocked_set &= ~(1U << sig); pending_array[sig] = 0; } else received[sig] = 0; for (sig = 0; sig < NSIG; sig++) if (received[sig]) raise (sig); } } return 0; } /* Install the handler FUNC for signal SIG, and return the previous handler. */ handler_t rpl_signal (int sig, handler_t handler) { /* We must provide a wrapper, so that a user can query what handler they installed even if that signal is currently blocked. */ if (sig >= 0 && sig < NSIG && sig != SIGKILL && sig != SIGSTOP && handler != SIG_ERR) { #ifdef SIGABRT_COMPAT if (sig == SIGABRT_COMPAT) sig = SIGABRT; #endif if (blocked_set & (1U << sig)) { /* POSIX states that sigprocmask and signal are both async-signal-safe. This is not true of our implementation - there is a slight data race where an asynchronous interrupt on signal A can occur after we install blocked_handler but before we have updated old_handlers for signal B, such that handler A can see stale information if it calls signal(B). Oh well - signal handlers really shouldn't try to manipulate the installed handlers of unrelated signals. */ handler_t result = old_handlers[sig]; old_handlers[sig] = handler; return result; } else return signal (sig, handler); } else { errno = EINVAL; return SIG_ERR; } } #if GNULIB_defined_SIGPIPE /* Raise the signal SIGPIPE. */ int _gl_raise_SIGPIPE (void) { if (blocked_set & (1U << SIGPIPE)) pending_array[SIGPIPE] = 1; else { handler_t handler = SIGPIPE_handler; if (handler == SIG_DFL) exit (128 + SIGPIPE); else if (handler != SIG_IGN) (*handler) (SIGPIPE); } return 0; } #endif gnuastro-0.5/bootstrapped/tests/signbitl.c0000644000175000017500000000414313217200023015760 00000000000000/* signbit() macro: Determine the sign bit of a floating-point number. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "isnanl-nolibm.h" #include "float+.h" #ifdef gl_signbitl_OPTIMIZED_MACRO # undef gl_signbitl #endif int gl_signbitl (long double arg) { #if defined LDBL_SIGNBIT_WORD && defined LDBL_SIGNBIT_BIT /* The use of a union to extract the bits of the representation of a 'long double' is safe in practice, despite of the "aliasing rules" of C99, because the GCC docs say "Even with '-fstrict-aliasing', type-punning is allowed, provided the memory is accessed through the union type." and similarly for other compilers. */ # define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) union { long double value; unsigned int word[NWORDS]; } m; m.value = arg; return (m.word[LDBL_SIGNBIT_WORD] >> LDBL_SIGNBIT_BIT) & 1; #elif HAVE_COPYSIGNL_IN_LIBC return copysignl (1.0L, arg) < 0; #else /* This does not do the right thing for NaN, but this is irrelevant for most use cases. */ if (isnanl (arg)) return 0; if (arg < 0.0L) return 1; else if (arg == 0.0L) { /* Distinguish 0.0L and -0.0L. */ static long double plus_zero = 0.0L; long double arg_mem = arg; return (memcmp (&plus_zero, &arg_mem, SIZEOF_LDBL) != 0); } else return 0; #endif } gnuastro-0.5/bootstrapped/tests/signbitf.c0000644000175000017500000000410013217200023015743 00000000000000/* signbit() macro: Determine the sign bit of a floating-point number. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "isnanf-nolibm.h" #include "float+.h" #ifdef gl_signbitf_OPTIMIZED_MACRO # undef gl_signbitf #endif int gl_signbitf (float arg) { #if defined FLT_SIGNBIT_WORD && defined FLT_SIGNBIT_BIT /* The use of a union to extract the bits of the representation of a 'long double' is safe in practice, despite of the "aliasing rules" of C99, because the GCC docs say "Even with '-fstrict-aliasing', type-punning is allowed, provided the memory is accessed through the union type." and similarly for other compilers. */ # define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) union { float value; unsigned int word[NWORDS]; } m; m.value = arg; return (m.word[FLT_SIGNBIT_WORD] >> FLT_SIGNBIT_BIT) & 1; #elif HAVE_COPYSIGNF_IN_LIBC return copysignf (1.0f, arg) < 0; #else /* This does not do the right thing for NaN, but this is irrelevant for most use cases. */ if (isnanf (arg)) return 0; if (arg < 0.0f) return 1; else if (arg == 0.0f) { /* Distinguish 0.0f and -0.0f. */ static float plus_zero = 0.0f; float arg_mem = arg; return (memcmp (&plus_zero, &arg_mem, SIZEOF_FLT) != 0); } else return 0; #endif } gnuastro-0.5/bootstrapped/tests/signbitd.c0000644000175000017500000000406713217200023015755 00000000000000/* signbit() macro: Determine the sign bit of a floating-point number. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "isnand-nolibm.h" #include "float+.h" #ifdef gl_signbitd_OPTIMIZED_MACRO # undef gl_signbitd #endif int gl_signbitd (double arg) { #if defined DBL_SIGNBIT_WORD && defined DBL_SIGNBIT_BIT /* The use of a union to extract the bits of the representation of a 'long double' is safe in practice, despite of the "aliasing rules" of C99, because the GCC docs say "Even with '-fstrict-aliasing', type-punning is allowed, provided the memory is accessed through the union type." and similarly for other compilers. */ # define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) union { double value; unsigned int word[NWORDS]; } m; m.value = arg; return (m.word[DBL_SIGNBIT_WORD] >> DBL_SIGNBIT_BIT) & 1; #elif HAVE_COPYSIGN_IN_LIBC return copysign (1.0, arg) < 0; #else /* This does not do the right thing for NaN, but this is irrelevant for most use cases. */ if (isnand (arg)) return 0; if (arg < 0.0) return 1; else if (arg == 0.0) { /* Distinguish 0.0 and -0.0. */ static double plus_zero = 0.0; double arg_mem = arg; return (memcmp (&plus_zero, &arg_mem, SIZEOF_DBL) != 0); } else return 0; #endif } gnuastro-0.5/bootstrapped/tests/sigaction.c0000644000175000017500000001614413217200023016131 00000000000000/* POSIX compatible signal blocking. Copyright (C) 2008-2017 Free Software Foundation, Inc. Written by Eric Blake , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include /* This implementation of sigaction is tailored to native Windows behavior: signal() has SysV semantics (ie. the handler is uninstalled before it is invoked). This is an inherent data race if an asynchronous signal is sent twice in a row before we can reinstall our handler, but there's nothing we can do about it. Meanwhile, sigprocmask() is not present, and while we can use the gnulib replacement to provide critical sections, it too suffers from potential data races in the face of an ill-timed asynchronous signal. And we compound the situation by reading static storage in a signal handler, which POSIX warns is not generically async-signal-safe. Oh well. Additionally: - We don't implement SA_NOCLDSTOP or SA_NOCLDWAIT, because SIGCHLD is not defined. - We don't implement SA_ONSTACK, because sigaltstack() is not present. - We ignore SA_RESTART, because blocking native Windows API calls are not interrupted anyway when an asynchronous signal occurs, and the MSVCRT runtime never sets errno to EINTR. - We don't implement SA_SIGINFO because it is impossible to do so portably. POSIX states that an application should not mix signal() and sigaction(). We support the use of signal() within the gnulib sigprocmask() substitute, but all other application code linked with this module should stick with only sigaction(). */ /* Check some of our assumptions. */ #if defined SIGCHLD || defined HAVE_SIGALTSTACK || defined HAVE_SIGINTERRUPT # error "Revisit the assumptions made in the sigaction module" #endif /* Out-of-range substitutes make a good fallback for uncatchable signals. */ #ifndef SIGKILL # define SIGKILL (-1) #endif #ifndef SIGSTOP # define SIGSTOP (-1) #endif /* On native Windows, as of 2008, the signal SIGABRT_COMPAT is an alias for the signal SIGABRT. Only one signal handler is stored for both SIGABRT and SIGABRT_COMPAT. SIGABRT_COMPAT is not a signal of its own. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # undef SIGABRT_COMPAT # define SIGABRT_COMPAT 6 #endif /* A signal handler. */ typedef void (*handler_t) (int signal); /* Set of current actions. If sa_handler for an entry is NULL, then that signal is not currently handled by the sigaction handler. */ static struct sigaction volatile action_array[NSIG] /* = 0 */; /* Signal handler that is installed for signals. */ static void sigaction_handler (int sig) { handler_t handler; sigset_t mask; sigset_t oldmask; int saved_errno = errno; if (sig < 0 || NSIG <= sig || !action_array[sig].sa_handler) { /* Unexpected situation; be careful to avoid recursive abort. */ if (sig == SIGABRT) signal (SIGABRT, SIG_DFL); abort (); } /* Reinstall the signal handler when required; otherwise update the bookkeeping so that the user's handler may call sigaction and get accurate results. We know the signal isn't currently blocked, or we wouldn't be in its handler, therefore we know that we are not interrupting a sigaction() call. There is a race where any asynchronous instance of the same signal occurring before we reinstall the handler will trigger the default handler; oh well. */ handler = action_array[sig].sa_handler; if ((action_array[sig].sa_flags & SA_RESETHAND) == 0) signal (sig, sigaction_handler); else action_array[sig].sa_handler = NULL; /* Block appropriate signals. */ mask = action_array[sig].sa_mask; if ((action_array[sig].sa_flags & SA_NODEFER) == 0) sigaddset (&mask, sig); sigprocmask (SIG_BLOCK, &mask, &oldmask); /* Invoke the user's handler, then restore prior mask. */ errno = saved_errno; handler (sig); saved_errno = errno; sigprocmask (SIG_SETMASK, &oldmask, NULL); errno = saved_errno; } /* Change and/or query the action that will be taken on delivery of signal SIG. If not NULL, ACT describes the new behavior. If not NULL, OACT is set to the prior behavior. Return 0 on success, or set errno and return -1 on failure. */ int sigaction (int sig, const struct sigaction *restrict act, struct sigaction *restrict oact) { sigset_t mask; sigset_t oldmask; int saved_errno; if (sig < 0 || NSIG <= sig || sig == SIGKILL || sig == SIGSTOP || (act && act->sa_handler == SIG_ERR)) { errno = EINVAL; return -1; } #ifdef SIGABRT_COMPAT if (sig == SIGABRT_COMPAT) sig = SIGABRT; #endif /* POSIX requires sigaction() to be async-signal-safe. In other words, if an asynchronous signal can occur while we are anywhere inside this function, the user's handler could then call sigaction() recursively and expect consistent results. We meet this rule by using sigprocmask to block all signals before modifying any data structure that could be read from a signal handler; this works since we know that the gnulib sigprocmask replacement does not try to use sigaction() from its handler. */ if (!act && !oact) return 0; sigfillset (&mask); sigprocmask (SIG_BLOCK, &mask, &oldmask); if (oact) { if (action_array[sig].sa_handler) *oact = action_array[sig]; else { /* Safe to change the handler at will here, since all signals are currently blocked. */ oact->sa_handler = signal (sig, SIG_DFL); if (oact->sa_handler == SIG_ERR) goto failure; signal (sig, oact->sa_handler); oact->sa_flags = SA_RESETHAND | SA_NODEFER; sigemptyset (&oact->sa_mask); } } if (act) { /* Safe to install the handler before updating action_array, since all signals are currently blocked. */ if (act->sa_handler == SIG_DFL || act->sa_handler == SIG_IGN) { if (signal (sig, act->sa_handler) == SIG_ERR) goto failure; action_array[sig].sa_handler = NULL; } else { if (signal (sig, sigaction_handler) == SIG_ERR) goto failure; action_array[sig] = *act; } } sigprocmask (SIG_SETMASK, &oldmask, NULL); return 0; failure: saved_errno = errno; sigprocmask (SIG_SETMASK, &oldmask, NULL); errno = saved_errno; return -1; } gnuastro-0.5/bootstrapped/tests/setsockopt.c0000644000175000017500000000334713217200023016350 00000000000000/* setsockopt.c --- wrappers for Windows setsockopt function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #define WIN32_LEAN_AND_MEAN /* Get winsock2.h. */ #include /* Get struct timeval. */ #include /* Get set_winsock_errno, FD_TO_SOCKET etc. */ #include "w32sock.h" #undef setsockopt int rpl_setsockopt (int fd, int level, int optname, const void *optval, socklen_t optlen) { SOCKET sock = FD_TO_SOCKET (fd); int r; if (sock == INVALID_SOCKET) { errno = EBADF; return -1; } else { if (level == SOL_SOCKET && (optname == SO_RCVTIMEO || optname == SO_SNDTIMEO)) { const struct timeval *tv = optval; int milliseconds = tv->tv_sec * 1000 + tv->tv_usec / 1000; optval = &milliseconds; r = setsockopt (sock, level, optname, optval, sizeof (int)); } else { r = setsockopt (sock, level, optname, optval, optlen); } if (r < 0) set_winsock_errno (); return r; } } gnuastro-0.5/bootstrapped/tests/setlocale.c0000644000175000017500000007054513217200023016131 00000000000000/* Set the current locale. -*- coding: utf-8 -*- Copyright (C) 2009, 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2009. */ #include /* Override setlocale() so that when the default locale is requested (locale = ""), the environment variables LC_ALL, LC_*, and LANG are considered. Also include all the functionality from libintl's setlocale() override. */ /* Please keep this file in sync with gettext/gettext-runtime/intl/setlocale.c ! */ /* Specification. */ #include #include #include #include "localename.h" #if 1 # undef setlocale /* Return string representation of locale category CATEGORY. */ static const char * category_to_name (int category) { const char *retval; switch (category) { case LC_COLLATE: retval = "LC_COLLATE"; break; case LC_CTYPE: retval = "LC_CTYPE"; break; case LC_MONETARY: retval = "LC_MONETARY"; break; case LC_NUMERIC: retval = "LC_NUMERIC"; break; case LC_TIME: retval = "LC_TIME"; break; case LC_MESSAGES: retval = "LC_MESSAGES"; break; default: /* If you have a better idea for a default value let me know. */ retval = "LC_XXX"; } return retval; } # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* The native Windows setlocale() function expects locale names of the form "German" or "German_Germany" or "DEU", but not "de" or "de_DE". We need to convert the names from the form with ISO 639 language code and ISO 3166 country code to the form with English names or with three-letter identifier. The three-letter identifiers known by a Windows XP SP2 or SP3 are: AFK Afrikaans_South Africa.1252 ARA Arabic_Saudi Arabia.1256 ARB Arabic_Lebanon.1256 ARE Arabic_Egypt.1256 ARG Arabic_Algeria.1256 ARH Arabic_Bahrain.1256 ARI Arabic_Iraq.1256 ARJ Arabic_Jordan.1256 ARK Arabic_Kuwait.1256 ARL Arabic_Libya.1256 ARM Arabic_Morocco.1256 ARO Arabic_Oman.1256 ARQ Arabic_Qatar.1256 ARS Arabic_Syria.1256 ART Arabic_Tunisia.1256 ARU Arabic_U.A.E..1256 ARY Arabic_Yemen.1256 AZE Azeri (Latin)_Azerbaijan.1254 BEL Belarusian_Belarus.1251 BGR Bulgarian_Bulgaria.1251 BSB Bosnian_Bosnia and Herzegovina.1250 BSC Bosnian (Cyrillic)_Bosnia and Herzegovina.1250 (wrong encoding!) CAT Catalan_Spain.1252 CHH Chinese_Hong Kong S.A.R..950 CHI Chinese_Singapore.936 CHS Chinese_People's Republic of China.936 CHT Chinese_Taiwan.950 CSY Czech_Czech Republic.1250 CYM Welsh_United Kingdom.1252 DAN Danish_Denmark.1252 DEA German_Austria.1252 DEC German_Liechtenstein.1252 DEL German_Luxembourg.1252 DES German_Switzerland.1252 DEU German_Germany.1252 ELL Greek_Greece.1253 ENA English_Australia.1252 ENB English_Caribbean.1252 ENC English_Canada.1252 ENG English_United Kingdom.1252 ENI English_Ireland.1252 ENJ English_Jamaica.1252 ENL English_Belize.1252 ENP English_Republic of the Philippines.1252 ENS English_South Africa.1252 ENT English_Trinidad and Tobago.1252 ENU English_United States.1252 ENW English_Zimbabwe.1252 ENZ English_New Zealand.1252 ESA Spanish_Panama.1252 ESB Spanish_Bolivia.1252 ESC Spanish_Costa Rica.1252 ESD Spanish_Dominican Republic.1252 ESE Spanish_El Salvador.1252 ESF Spanish_Ecuador.1252 ESG Spanish_Guatemala.1252 ESH Spanish_Honduras.1252 ESI Spanish_Nicaragua.1252 ESL Spanish_Chile.1252 ESM Spanish_Mexico.1252 ESN Spanish_Spain.1252 ESO Spanish_Colombia.1252 ESP Spanish_Spain.1252 ESR Spanish_Peru.1252 ESS Spanish_Argentina.1252 ESU Spanish_Puerto Rico.1252 ESV Spanish_Venezuela.1252 ESY Spanish_Uruguay.1252 ESZ Spanish_Paraguay.1252 ETI Estonian_Estonia.1257 EUQ Basque_Spain.1252 FAR Farsi_Iran.1256 FIN Finnish_Finland.1252 FOS Faroese_Faroe Islands.1252 FPO Filipino_Philippines.1252 FRA French_France.1252 FRB French_Belgium.1252 FRC French_Canada.1252 FRL French_Luxembourg.1252 FRM French_Principality of Monaco.1252 FRS French_Switzerland.1252 FYN Frisian_Netherlands.1252 GLC Galician_Spain.1252 HEB Hebrew_Israel.1255 HRB Croatian_Bosnia and Herzegovina.1250 HRV Croatian_Croatia.1250 HUN Hungarian_Hungary.1250 IND Indonesian_Indonesia.1252 IRE Irish_Ireland.1252 ISL Icelandic_Iceland.1252 ITA Italian_Italy.1252 ITS Italian_Switzerland.1252 IUK Inuktitut (Latin)_Canada.1252 JPN Japanese_Japan.932 KKZ Kazakh_Kazakhstan.1251 KOR Korean_Korea.949 KYR Kyrgyz_Kyrgyzstan.1251 LBX Luxembourgish_Luxembourg.1252 LTH Lithuanian_Lithuania.1257 LVI Latvian_Latvia.1257 MKI FYRO Macedonian_Former Yugoslav Republic of Macedonia.1251 MON Mongolian_Mongolia.1251 MPD Mapudungun_Chile.1252 MSB Malay_Brunei Darussalam.1252 MSL Malay_Malaysia.1252 MWK Mohawk_Canada.1252 NLB Dutch_Belgium.1252 NLD Dutch_Netherlands.1252 NON Norwegian-Nynorsk_Norway.1252 NOR Norwegian (BokmÃ¥l)_Norway.1252 NSO Northern Sotho_South Africa.1252 PLK Polish_Poland.1250 PTB Portuguese_Brazil.1252 PTG Portuguese_Portugal.1252 QUB Quechua_Bolivia.1252 QUE Quechua_Ecuador.1252 QUP Quechua_Peru.1252 RMC Romansh_Switzerland.1252 ROM Romanian_Romania.1250 RUS Russian_Russia.1251 SKY Slovak_Slovakia.1250 SLV Slovenian_Slovenia.1250 SMA Sami (Southern)_Norway.1252 SMB Sami (Southern)_Sweden.1252 SME Sami (Northern)_Norway.1252 SMF Sami (Northern)_Sweden.1252 SMG Sami (Northern)_Finland.1252 SMJ Sami (Lule)_Norway.1252 SMK Sami (Lule)_Sweden.1252 SMN Sami (Inari)_Finland.1252 SMS Sami (Skolt)_Finland.1252 SQI Albanian_Albania.1250 SRB Serbian (Cyrillic)_Serbia and Montenegro.1251 SRL Serbian (Latin)_Serbia and Montenegro.1250 SRN Serbian (Cyrillic)_Bosnia and Herzegovina.1251 SRS Serbian (Latin)_Bosnia and Herzegovina.1250 SVE Swedish_Sweden.1252 SVF Swedish_Finland.1252 SWK Swahili_Kenya.1252 THA Thai_Thailand.874 TRK Turkish_Turkey.1254 TSN Tswana_South Africa.1252 TTT Tatar_Russia.1251 UKR Ukrainian_Ukraine.1251 URD Urdu_Islamic Republic of Pakistan.1256 USA English_United States.1252 UZB Uzbek (Latin)_Uzbekistan.1254 VIT Vietnamese_Viet Nam.1258 XHO Xhosa_South Africa.1252 ZHH Chinese_Hong Kong S.A.R..950 ZHI Chinese_Singapore.936 ZHM Chinese_Macau S.A.R..950 ZUL Zulu_South Africa.1252 */ /* Table from ISO 639 language code, optionally with country or script suffix, to English name. Keep in sync with the gl_locale_name_from_win32_LANGID function in localename.c! */ struct table_entry { const char *code; const char *english; }; static const struct table_entry language_table[] = { { "af", "Afrikaans" }, { "am", "Amharic" }, { "ar", "Arabic" }, { "arn", "Mapudungun" }, { "as", "Assamese" }, { "az@cyrillic", "Azeri (Cyrillic)" }, { "az@latin", "Azeri (Latin)" }, { "ba", "Bashkir" }, { "be", "Belarusian" }, { "ber", "Tamazight" }, { "ber@arabic", "Tamazight (Arabic)" }, { "ber@latin", "Tamazight (Latin)" }, { "bg", "Bulgarian" }, { "bin", "Edo" }, { "bn", "Bengali" }, { "bn_BD", "Bengali (Bangladesh)" }, { "bn_IN", "Bengali (India)" }, { "bnt", "Sutu" }, { "bo", "Tibetan" }, { "br", "Breton" }, { "bs", "BSB" }, /* "Bosnian (Latin)" */ { "bs@cyrillic", "BSC" }, /* Bosnian (Cyrillic) */ { "ca", "Catalan" }, { "chr", "Cherokee" }, { "co", "Corsican" }, { "cpe", "Hawaiian" }, { "cs", "Czech" }, { "cy", "Welsh" }, { "da", "Danish" }, { "de", "German" }, { "dsb", "Lower Sorbian" }, { "dv", "Divehi" }, { "el", "Greek" }, { "en", "English" }, { "es", "Spanish" }, { "et", "Estonian" }, { "eu", "Basque" }, { "fa", "Farsi" }, { "ff", "Fulfulde" }, { "fi", "Finnish" }, { "fo", "Faroese" }, /* "Faeroese" does not work */ { "fr", "French" }, { "fy", "Frisian" }, { "ga", "IRE" }, /* Gaelic (Ireland) */ { "gd", "Gaelic (Scotland)" }, { "gd", "Scottish Gaelic" }, { "gl", "Galician" }, { "gn", "Guarani" }, { "gsw", "Alsatian" }, { "gu", "Gujarati" }, { "ha", "Hausa" }, { "he", "Hebrew" }, { "hi", "Hindi" }, { "hr", "Croatian" }, { "hsb", "Upper Sorbian" }, { "hu", "Hungarian" }, { "hy", "Armenian" }, { "id", "Indonesian" }, { "ig", "Igbo" }, { "ii", "Yi" }, { "is", "Icelandic" }, { "it", "Italian" }, { "iu", "IUK" }, /* Inuktitut */ { "ja", "Japanese" }, { "ka", "Georgian" }, { "kk", "Kazakh" }, { "kl", "Greenlandic" }, { "km", "Cambodian" }, { "km", "Khmer" }, { "kn", "Kannada" }, { "ko", "Korean" }, { "kok", "Konkani" }, { "kr", "Kanuri" }, { "ks", "Kashmiri" }, { "ks_IN", "Kashmiri_India" }, { "ks_PK", "Kashmiri (Arabic)_Pakistan" }, { "ky", "Kyrgyz" }, { "la", "Latin" }, { "lb", "Luxembourgish" }, { "lo", "Lao" }, { "lt", "Lithuanian" }, { "lv", "Latvian" }, { "mi", "Maori" }, { "mk", "FYRO Macedonian" }, { "mk", "Macedonian" }, { "ml", "Malayalam" }, { "mn", "Mongolian" }, { "mni", "Manipuri" }, { "moh", "Mohawk" }, { "mr", "Marathi" }, { "ms", "Malay" }, { "mt", "Maltese" }, { "my", "Burmese" }, { "nb", "NOR" }, /* Norwegian BokmÃ¥l */ { "ne", "Nepali" }, { "nic", "Ibibio" }, { "nl", "Dutch" }, { "nn", "NON" }, /* Norwegian Nynorsk */ { "no", "Norwegian" }, { "nso", "Northern Sotho" }, { "nso", "Sepedi" }, { "oc", "Occitan" }, { "om", "Oromo" }, { "or", "Oriya" }, { "pa", "Punjabi" }, { "pap", "Papiamentu" }, { "pl", "Polish" }, { "prs", "Dari" }, { "ps", "Pashto" }, { "pt", "Portuguese" }, { "qu", "Quechua" }, { "qut", "K'iche'" }, { "rm", "Romansh" }, { "ro", "Romanian" }, { "ru", "Russian" }, { "rw", "Kinyarwanda" }, { "sa", "Sanskrit" }, { "sah", "Yakut" }, { "sd", "Sindhi" }, { "se", "Sami (Northern)" }, { "se", "Northern Sami" }, { "si", "Sinhalese" }, { "sk", "Slovak" }, { "sl", "Slovenian" }, { "sma", "Sami (Southern)" }, { "sma", "Southern Sami" }, { "smj", "Sami (Lule)" }, { "smj", "Lule Sami" }, { "smn", "Sami (Inari)" }, { "smn", "Inari Sami" }, { "sms", "Sami (Skolt)" }, { "sms", "Skolt Sami" }, { "so", "Somali" }, { "sq", "Albanian" }, { "sr", "Serbian (Latin)" }, { "sr@cyrillic", "SRB" }, /* Serbian (Cyrillic) */ { "sv", "Swedish" }, { "sw", "Swahili" }, { "syr", "Syriac" }, { "ta", "Tamil" }, { "te", "Telugu" }, { "tg", "Tajik" }, { "th", "Thai" }, { "ti", "Tigrinya" }, { "tk", "Turkmen" }, { "tl", "Filipino" }, { "tn", "Tswana" }, { "tr", "Turkish" }, { "ts", "Tsonga" }, { "tt", "Tatar" }, { "ug", "Uighur" }, { "uk", "Ukrainian" }, { "ur", "Urdu" }, { "uz", "Uzbek" }, { "uz", "Uzbek (Latin)" }, { "uz@cyrillic", "Uzbek (Cyrillic)" }, { "ve", "Venda" }, { "vi", "Vietnamese" }, { "wen", "Sorbian" }, { "wo", "Wolof" }, { "xh", "Xhosa" }, { "yi", "Yiddish" }, { "yo", "Yoruba" }, { "zh", "Chinese" }, { "zu", "Zulu" } }; /* Table from ISO 3166 country code to English name. Keep in sync with the gl_locale_name_from_win32_LANGID function in localename.c! */ static const struct table_entry country_table[] = { { "AE", "U.A.E." }, { "AF", "Afghanistan" }, { "AL", "Albania" }, { "AM", "Armenia" }, { "AN", "Netherlands Antilles" }, { "AR", "Argentina" }, { "AT", "Austria" }, { "AU", "Australia" }, { "AZ", "Azerbaijan" }, { "BA", "Bosnia and Herzegovina" }, { "BD", "Bangladesh" }, { "BE", "Belgium" }, { "BG", "Bulgaria" }, { "BH", "Bahrain" }, { "BN", "Brunei Darussalam" }, { "BO", "Bolivia" }, { "BR", "Brazil" }, { "BT", "Bhutan" }, { "BY", "Belarus" }, { "BZ", "Belize" }, { "CA", "Canada" }, { "CG", "Congo" }, { "CH", "Switzerland" }, { "CI", "Cote d'Ivoire" }, { "CL", "Chile" }, { "CM", "Cameroon" }, { "CN", "People's Republic of China" }, { "CO", "Colombia" }, { "CR", "Costa Rica" }, { "CS", "Serbia and Montenegro" }, { "CZ", "Czech Republic" }, { "DE", "Germany" }, { "DK", "Denmark" }, { "DO", "Dominican Republic" }, { "DZ", "Algeria" }, { "EC", "Ecuador" }, { "EE", "Estonia" }, { "EG", "Egypt" }, { "ER", "Eritrea" }, { "ES", "Spain" }, { "ET", "Ethiopia" }, { "FI", "Finland" }, { "FO", "Faroe Islands" }, { "FR", "France" }, { "GB", "United Kingdom" }, { "GD", "Caribbean" }, { "GE", "Georgia" }, { "GL", "Greenland" }, { "GR", "Greece" }, { "GT", "Guatemala" }, { "HK", "Hong Kong" }, { "HK", "Hong Kong S.A.R." }, { "HN", "Honduras" }, { "HR", "Croatia" }, { "HT", "Haiti" }, { "HU", "Hungary" }, { "ID", "Indonesia" }, { "IE", "Ireland" }, { "IL", "Israel" }, { "IN", "India" }, { "IQ", "Iraq" }, { "IR", "Iran" }, { "IS", "Iceland" }, { "IT", "Italy" }, { "JM", "Jamaica" }, { "JO", "Jordan" }, { "JP", "Japan" }, { "KE", "Kenya" }, { "KG", "Kyrgyzstan" }, { "KH", "Cambodia" }, { "KR", "South Korea" }, { "KW", "Kuwait" }, { "KZ", "Kazakhstan" }, { "LA", "Laos" }, { "LB", "Lebanon" }, { "LI", "Liechtenstein" }, { "LK", "Sri Lanka" }, { "LT", "Lithuania" }, { "LU", "Luxembourg" }, { "LV", "Latvia" }, { "LY", "Libya" }, { "MA", "Morocco" }, { "MC", "Principality of Monaco" }, { "MD", "Moldava" }, { "MD", "Moldova" }, { "ME", "Montenegro" }, { "MK", "Former Yugoslav Republic of Macedonia" }, { "ML", "Mali" }, { "MM", "Myanmar" }, { "MN", "Mongolia" }, { "MO", "Macau S.A.R." }, { "MT", "Malta" }, { "MV", "Maldives" }, { "MX", "Mexico" }, { "MY", "Malaysia" }, { "NG", "Nigeria" }, { "NI", "Nicaragua" }, { "NL", "Netherlands" }, { "NO", "Norway" }, { "NP", "Nepal" }, { "NZ", "New Zealand" }, { "OM", "Oman" }, { "PA", "Panama" }, { "PE", "Peru" }, { "PH", "Philippines" }, { "PK", "Islamic Republic of Pakistan" }, { "PL", "Poland" }, { "PR", "Puerto Rico" }, { "PT", "Portugal" }, { "PY", "Paraguay" }, { "QA", "Qatar" }, { "RE", "Reunion" }, { "RO", "Romania" }, { "RS", "Serbia" }, { "RU", "Russia" }, { "RW", "Rwanda" }, { "SA", "Saudi Arabia" }, { "SE", "Sweden" }, { "SG", "Singapore" }, { "SI", "Slovenia" }, { "SK", "Slovak" }, { "SN", "Senegal" }, { "SO", "Somalia" }, { "SR", "Suriname" }, { "SV", "El Salvador" }, { "SY", "Syria" }, { "TH", "Thailand" }, { "TJ", "Tajikistan" }, { "TM", "Turkmenistan" }, { "TN", "Tunisia" }, { "TR", "Turkey" }, { "TT", "Trinidad and Tobago" }, { "TW", "Taiwan" }, { "TZ", "Tanzania" }, { "UA", "Ukraine" }, { "US", "United States" }, { "UY", "Uruguay" }, { "VA", "Vatican" }, { "VE", "Venezuela" }, { "VN", "Viet Nam" }, { "YE", "Yemen" }, { "ZA", "South Africa" }, { "ZW", "Zimbabwe" } }; /* Given a string STRING, find the set of indices i such that TABLE[i].code is the given STRING. It is a range [lo,hi-1]. */ typedef struct { size_t lo; size_t hi; } range_t; static void search (const struct table_entry *table, size_t table_size, const char *string, range_t *result) { /* The table is sorted. Perform a binary search. */ size_t hi = table_size; size_t lo = 0; while (lo < hi) { /* Invariant: for i < lo, strcmp (table[i].code, string) < 0, for i >= hi, strcmp (table[i].code, string) > 0. */ size_t mid = (hi + lo) >> 1; /* >= lo, < hi */ int cmp = strcmp (table[mid].code, string); if (cmp < 0) lo = mid + 1; else if (cmp > 0) hi = mid; else { /* Found an i with strcmp (language_table[i].code, string) == 0. Find the entire interval of such i. */ { size_t i; for (i = mid; i > lo; ) { i--; if (strcmp (table[i].code, string) < 0) { lo = i + 1; break; } } } { size_t i; for (i = mid; i < hi; i++) { if (strcmp (table[i].code, string) > 0) { hi = i; break; } } } /* The set of i with strcmp (language_table[i].code, string) == 0 is the interval [lo, hi-1]. */ break; } } result->lo = lo; result->hi = hi; } /* Like setlocale, but accept also locale names in the form ll or ll_CC, where ll is an ISO 639 language code and CC is an ISO 3166 country code. */ static char * setlocale_unixlike (int category, const char *locale) { char *result; char llCC_buf[64]; char ll_buf[64]; char CC_buf[64]; /* The native Windows implementation of setlocale understands the special locale name "C", but not "POSIX". Therefore map "POSIX" to "C". */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ if (locale != NULL && strcmp (locale, "POSIX") == 0) locale = "C"; #endif /* First, try setlocale with the original argument unchanged. */ result = setlocale (category, locale); if (result != NULL) return result; /* Otherwise, assume the argument is in the form language[_territory][.codeset][@modifier] and try to map it using the tables. */ if (strlen (locale) < sizeof (llCC_buf)) { /* Second try: Remove the codeset part. */ { const char *p = locale; char *q = llCC_buf; /* Copy the part before the dot. */ for (; *p != '\0' && *p != '.'; p++, q++) *q = *p; if (*p == '.') /* Skip the part up to the '@', if any. */ for (; *p != '\0' && *p != '@'; p++) ; /* Copy the part starting with '@', if any. */ for (; *p != '\0'; p++, q++) *q = *p; *q = '\0'; } /* llCC_buf now contains language[_territory][@modifier] */ if (strcmp (llCC_buf, locale) != 0) { result = setlocale (category, llCC_buf); if (result != NULL) return result; } /* Look it up in language_table. */ { range_t range; size_t i; search (language_table, sizeof (language_table) / sizeof (language_table[0]), llCC_buf, &range); for (i = range.lo; i < range.hi; i++) { /* Try the replacement in language_table[i]. */ result = setlocale (category, language_table[i].english); if (result != NULL) return result; } } /* Split language[_territory][@modifier] into ll_buf = language[@modifier] and CC_buf = territory */ { const char *underscore = strchr (llCC_buf, '_'); if (underscore != NULL) { const char *territory_start = underscore + 1; const char *territory_end = strchr (territory_start, '@'); if (territory_end == NULL) territory_end = territory_start + strlen (territory_start); memcpy (ll_buf, llCC_buf, underscore - llCC_buf); strcpy (ll_buf + (underscore - llCC_buf), territory_end); memcpy (CC_buf, territory_start, territory_end - territory_start); CC_buf[territory_end - territory_start] = '\0'; { /* Look up ll_buf in language_table and CC_buf in country_table. */ range_t language_range; search (language_table, sizeof (language_table) / sizeof (language_table[0]), ll_buf, &language_range); if (language_range.lo < language_range.hi) { range_t country_range; search (country_table, sizeof (country_table) / sizeof (country_table[0]), CC_buf, &country_range); if (country_range.lo < country_range.hi) { size_t i; size_t j; for (i = language_range.lo; i < language_range.hi; i++) for (j = country_range.lo; j < country_range.hi; j++) { /* Concatenate the replacements. */ const char *part1 = language_table[i].english; size_t part1_len = strlen (part1); const char *part2 = country_table[j].english; size_t part2_len = strlen (part2) + 1; char buf[64+64]; if (!(part1_len + 1 + part2_len <= sizeof (buf))) abort (); memcpy (buf, part1, part1_len); buf[part1_len] = '_'; memcpy (buf + part1_len + 1, part2, part2_len); /* Try the concatenated replacements. */ result = setlocale (category, buf); if (result != NULL) return result; } } /* Try omitting the country entirely. This may set a locale corresponding to the wrong country, but is better than failing entirely. */ { size_t i; for (i = language_range.lo; i < language_range.hi; i++) { /* Try only the language replacement. */ result = setlocale (category, language_table[i].english); if (result != NULL) return result; } } } } } } } /* Failed. */ return NULL; } # else # define setlocale_unixlike setlocale # endif # if LC_MESSAGES == 1729 /* The system does not store an LC_MESSAGES locale category. Do it here. */ static char lc_messages_name[64] = "C"; /* Like setlocale, but support also LC_MESSAGES. */ static char * setlocale_single (int category, const char *locale) { if (category == LC_MESSAGES) { if (locale != NULL) { lc_messages_name[sizeof (lc_messages_name) - 1] = '\0'; strncpy (lc_messages_name, locale, sizeof (lc_messages_name) - 1); } return lc_messages_name; } else return setlocale_unixlike (category, locale); } # else # define setlocale_single setlocale_unixlike # endif char * rpl_setlocale (int category, const char *locale) { if (locale != NULL && locale[0] == '\0') { /* A request to the set the current locale to the default locale. */ if (category == LC_ALL) { /* Set LC_CTYPE first. Then the other categories. */ static int const categories[] = { LC_NUMERIC, LC_TIME, LC_COLLATE, LC_MONETARY, LC_MESSAGES }; char *saved_locale; const char *base_name; unsigned int i; /* Back up the old locale, in case one of the steps fails. */ saved_locale = setlocale (LC_ALL, NULL); if (saved_locale == NULL) return NULL; saved_locale = strdup (saved_locale); if (saved_locale == NULL) return NULL; /* Set LC_CTYPE category. Set all other categories (except possibly LC_MESSAGES) to the same value in the same call; this is likely to save calls. */ base_name = gl_locale_name_environ (LC_CTYPE, category_to_name (LC_CTYPE)); if (base_name == NULL) base_name = gl_locale_name_default (); if (setlocale_unixlike (LC_ALL, base_name) == NULL) goto fail; # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, setlocale(LC_ALL,...) may succeed but set the LC_CTYPE category to an invalid value ("C") when it does not support the specified encoding. Report a failure instead. */ if (strchr (base_name, '.') != NULL && strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) goto fail; # endif for (i = 0; i < sizeof (categories) / sizeof (categories[0]); i++) { int cat = categories[i]; const char *name; name = gl_locale_name_environ (cat, category_to_name (cat)); if (name == NULL) name = gl_locale_name_default (); /* If name is the same as base_name, it has already been set through the setlocale call before the loop. */ if (strcmp (name, base_name) != 0 # if LC_MESSAGES == 1729 || cat == LC_MESSAGES # endif ) if (setlocale_single (cat, name) == NULL) goto fail; } /* All steps were successful. */ free (saved_locale); return setlocale (LC_ALL, NULL); fail: if (saved_locale[0] != '\0') /* don't risk an endless recursion */ setlocale (LC_ALL, saved_locale); free (saved_locale); return NULL; } else { const char *name = gl_locale_name_environ (category, category_to_name (category)); if (name == NULL) name = gl_locale_name_default (); return setlocale_single (category, name); } } else { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ if (category == LC_ALL && locale != NULL && strchr (locale, '.') != NULL) { char *saved_locale; /* Back up the old locale. */ saved_locale = setlocale (LC_ALL, NULL); if (saved_locale == NULL) return NULL; saved_locale = strdup (saved_locale); if (saved_locale == NULL) return NULL; if (setlocale_unixlike (LC_ALL, locale) == NULL) { free (saved_locale); return NULL; } /* On native Windows, setlocale(LC_ALL,...) may succeed but set the LC_CTYPE category to an invalid value ("C") when it does not support the specified encoding. Report a failure instead. */ if (strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) { if (saved_locale[0] != '\0') /* don't risk an endless recursion */ setlocale (LC_ALL, saved_locale); free (saved_locale); return NULL; } /* It was really successful. */ free (saved_locale); return setlocale (LC_ALL, NULL); } else # endif return setlocale_single (category, locale); } } #endif gnuastro-0.5/bootstrapped/tests/setenv.c0000644000175000017500000002502713217200023015455 00000000000000/* Copyright (C) 1992, 1995-2003, 2005-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if !_LIBC /* Don't use __attribute__ __nonnull__ in this compilation unit. Otherwise gcc optimizes away the name == NULL test below. */ # define _GL_ARG_NONNULL(params) # define _GL_USE_STDLIB_ALLOC 1 # include #endif #include /* Specification. */ #include #include #ifndef __set_errno # define __set_errno(ev) ((errno) = (ev)) #endif #include #if _LIBC || HAVE_UNISTD_H # include #endif #if !_LIBC # include "malloca.h" #endif #if _LIBC || !HAVE_SETENV #if !_LIBC # define __environ environ #endif #if _LIBC /* This lock protects against simultaneous modifications of 'environ'. */ # include __libc_lock_define_initialized (static, envlock) # define LOCK __libc_lock_lock (envlock) # define UNLOCK __libc_lock_unlock (envlock) #else # define LOCK # define UNLOCK #endif /* In the GNU C library we must keep the namespace clean. */ #ifdef _LIBC # define setenv __setenv # define clearenv __clearenv # define tfind __tfind # define tsearch __tsearch #endif /* In the GNU C library implementation we try to be more clever and allow arbitrarily many changes of the environment given that the used values are from a small set. Outside glibc this will eat up all memory after a while. */ #if defined _LIBC || (defined HAVE_SEARCH_H && defined HAVE_TSEARCH \ && defined __GNUC__) # define USE_TSEARCH 1 # include typedef int (*compar_fn_t) (const void *, const void *); /* This is a pointer to the root of the search tree with the known values. */ static void *known_values; # define KNOWN_VALUE(Str) \ ({ \ void *value = tfind (Str, &known_values, (compar_fn_t) strcmp); \ value != NULL ? *(char **) value : NULL; \ }) # define STORE_VALUE(Str) \ tsearch (Str, &known_values, (compar_fn_t) strcmp) #else # undef USE_TSEARCH # define KNOWN_VALUE(Str) NULL # define STORE_VALUE(Str) do { } while (0) #endif /* If this variable is not a null pointer we allocated the current environment. */ static char **last_environ; /* This function is used by 'setenv' and 'putenv'. The difference between the two functions is that for the former must create a new string which is then placed in the environment, while the argument of 'putenv' must be used directly. This is all complicated by the fact that we try to reuse values once generated for a 'setenv' call since we can never free the strings. */ int __add_to_environ (const char *name, const char *value, const char *combined, int replace) { char **ep; size_t size; const size_t namelen = strlen (name); const size_t vallen = value != NULL ? strlen (value) + 1 : 0; LOCK; /* We have to get the pointer now that we have the lock and not earlier since another thread might have created a new environment. */ ep = __environ; size = 0; if (ep != NULL) { for (; *ep != NULL; ++ep) if (!strncmp (*ep, name, namelen) && (*ep)[namelen] == '=') break; else ++size; } if (ep == NULL || *ep == NULL) { char **new_environ; #ifdef USE_TSEARCH char *new_value; #endif /* We allocated this space; we can extend it. */ new_environ = (char **) (last_environ == NULL ? malloc ((size + 2) * sizeof (char *)) : realloc (last_environ, (size + 2) * sizeof (char *))); if (new_environ == NULL) { /* It's easier to set errno to ENOMEM than to rely on the 'malloc-posix' and 'realloc-posix' gnulib modules. */ __set_errno (ENOMEM); UNLOCK; return -1; } /* If the whole entry is given add it. */ if (combined != NULL) /* We must not add the string to the search tree since it belongs to the user. */ new_environ[size] = (char *) combined; else { /* See whether the value is already known. */ #ifdef USE_TSEARCH # ifdef _LIBC new_value = (char *) alloca (namelen + 1 + vallen); __mempcpy (__mempcpy (__mempcpy (new_value, name, namelen), "=", 1), value, vallen); # else new_value = (char *) malloca (namelen + 1 + vallen); if (new_value == NULL) { __set_errno (ENOMEM); UNLOCK; return -1; } memcpy (new_value, name, namelen); new_value[namelen] = '='; memcpy (&new_value[namelen + 1], value, vallen); # endif new_environ[size] = KNOWN_VALUE (new_value); if (new_environ[size] == NULL) #endif { new_environ[size] = (char *) malloc (namelen + 1 + vallen); if (new_environ[size] == NULL) { #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif __set_errno (ENOMEM); UNLOCK; return -1; } #ifdef USE_TSEARCH memcpy (new_environ[size], new_value, namelen + 1 + vallen); #else memcpy (new_environ[size], name, namelen); new_environ[size][namelen] = '='; memcpy (&new_environ[size][namelen + 1], value, vallen); #endif /* And save the value now. We cannot do this when we remove the string since then we cannot decide whether it is a user string or not. */ STORE_VALUE (new_environ[size]); } #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif } if (__environ != last_environ) memcpy ((char *) new_environ, (char *) __environ, size * sizeof (char *)); new_environ[size + 1] = NULL; last_environ = __environ = new_environ; } else if (replace) { char *np; /* Use the user string if given. */ if (combined != NULL) np = (char *) combined; else { #ifdef USE_TSEARCH char *new_value; # ifdef _LIBC new_value = alloca (namelen + 1 + vallen); __mempcpy (__mempcpy (__mempcpy (new_value, name, namelen), "=", 1), value, vallen); # else new_value = malloca (namelen + 1 + vallen); if (new_value == NULL) { __set_errno (ENOMEM); UNLOCK; return -1; } memcpy (new_value, name, namelen); new_value[namelen] = '='; memcpy (&new_value[namelen + 1], value, vallen); # endif np = KNOWN_VALUE (new_value); if (np == NULL) #endif { np = (char *) malloc (namelen + 1 + vallen); if (np == NULL) { #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif __set_errno (ENOMEM); UNLOCK; return -1; } #ifdef USE_TSEARCH memcpy (np, new_value, namelen + 1 + vallen); #else memcpy (np, name, namelen); np[namelen] = '='; memcpy (&np[namelen + 1], value, vallen); #endif /* And remember the value. */ STORE_VALUE (np); } #if defined USE_TSEARCH && !defined _LIBC freea (new_value); #endif } *ep = np; } UNLOCK; return 0; } int setenv (const char *name, const char *value, int replace) { if (name == NULL || *name == '\0' || strchr (name, '=') != NULL) { __set_errno (EINVAL); return -1; } return __add_to_environ (name, value, NULL, replace); } /* The 'clearenv' was planned to be added to POSIX.1 but probably never made it. Nevertheless the POSIX.9 standard (POSIX bindings for Fortran 77) requires this function. */ int clearenv (void) { LOCK; if (__environ == last_environ && __environ != NULL) { /* We allocated this environment so we can free it. */ free (__environ); last_environ = NULL; } /* Clear the environment pointer removes the whole environment. */ __environ = NULL; UNLOCK; return 0; } #ifdef _LIBC static void free_mem (void) { /* Remove all traces. */ clearenv (); /* Now remove the search tree. */ __tdestroy (known_values, free); known_values = NULL; } text_set_element (__libc_subfreeres, free_mem); # undef setenv # undef clearenv weak_alias (__setenv, setenv) weak_alias (__clearenv, clearenv) #endif #endif /* _LIBC || !HAVE_SETENV */ /* The rest of this file is called into use when replacing an existing but buggy setenv. Known bugs include failure to diagnose invalid name, and consuming a leading '=' from value. */ #if HAVE_SETENV # undef setenv # if !HAVE_DECL_SETENV extern int setenv (const char *, const char *, int); # endif # define STREQ(a, b) (strcmp (a, b) == 0) int rpl_setenv (const char *name, const char *value, int replace) { int result; if (!name || !*name || strchr (name, '=')) { errno = EINVAL; return -1; } /* Call the real setenv even if replace is 0, in case implementation has underlying data to update, such as when environ changes. */ result = setenv (name, value, replace); if (result == 0 && replace && *value == '=') { char *tmp = getenv (name); if (!STREQ (tmp, value)) { int saved_errno; size_t len = strlen (value); tmp = malloca (len + 2); /* Since leading '=' is eaten, double it up. */ *tmp = '='; memcpy (tmp + 1, value, len + 1); result = setenv (name, tmp, replace); saved_errno = errno; freea (tmp); errno = saved_errno; } } return result; } #endif /* HAVE_SETENV */ gnuastro-0.5/bootstrapped/tests/select.c0000644000175000017500000003771113217200023015433 00000000000000/* Emulation for select(2) Contributed by Paolo Bonzini. Copyright 2008-2017 Free Software Foundation, Inc. This file is part of gnulib. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Native Windows. */ #include #include #include #include #include #include #include #include #include /* Get the overridden 'struct timeval'. */ #include #if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" #else # include #endif #undef select struct bitset { unsigned char in[FD_SETSIZE / CHAR_BIT]; unsigned char out[FD_SETSIZE / CHAR_BIT]; }; /* Declare data structures for ntdll functions. */ typedef struct _FILE_PIPE_LOCAL_INFORMATION { ULONG NamedPipeType; ULONG NamedPipeConfiguration; ULONG MaximumInstances; ULONG CurrentInstances; ULONG InboundQuota; ULONG ReadDataAvailable; ULONG OutboundQuota; ULONG WriteQuotaAvailable; ULONG NamedPipeState; ULONG NamedPipeEnd; } FILE_PIPE_LOCAL_INFORMATION, *PFILE_PIPE_LOCAL_INFORMATION; typedef struct _IO_STATUS_BLOCK { union { DWORD Status; PVOID Pointer; } u; ULONG_PTR Information; } IO_STATUS_BLOCK, *PIO_STATUS_BLOCK; typedef enum _FILE_INFORMATION_CLASS { FilePipeLocalInformation = 24 } FILE_INFORMATION_CLASS, *PFILE_INFORMATION_CLASS; typedef DWORD (WINAPI *PNtQueryInformationFile) (HANDLE, IO_STATUS_BLOCK *, VOID *, ULONG, FILE_INFORMATION_CLASS); #ifndef PIPE_BUF #define PIPE_BUF 512 #endif static BOOL IsConsoleHandle (HANDLE h) { DWORD mode; return GetConsoleMode (h, &mode) != 0; } static BOOL IsSocketHandle (HANDLE h) { WSANETWORKEVENTS ev; if (IsConsoleHandle (h)) return FALSE; /* Under Wine, it seems that getsockopt returns 0 for pipes too. WSAEnumNetworkEvents instead distinguishes the two correctly. */ ev.lNetworkEvents = 0xDEADBEEF; WSAEnumNetworkEvents ((SOCKET) h, NULL, &ev); return ev.lNetworkEvents != 0xDEADBEEF; } /* Compute output fd_sets for libc descriptor FD (whose Windows handle is H). */ static int windows_poll_handle (HANDLE h, int fd, struct bitset *rbits, struct bitset *wbits, struct bitset *xbits) { BOOL read, write, except; int i, ret; INPUT_RECORD *irbuffer; DWORD avail, nbuffer; BOOL bRet; IO_STATUS_BLOCK iosb; FILE_PIPE_LOCAL_INFORMATION fpli; static PNtQueryInformationFile NtQueryInformationFile; static BOOL once_only; read = write = except = FALSE; switch (GetFileType (h)) { case FILE_TYPE_DISK: read = TRUE; write = TRUE; break; case FILE_TYPE_PIPE: if (!once_only) { NtQueryInformationFile = (PNtQueryInformationFile) GetProcAddress (GetModuleHandle ("ntdll.dll"), "NtQueryInformationFile"); once_only = TRUE; } if (PeekNamedPipe (h, NULL, 0, NULL, &avail, NULL) != 0) { if (avail) read = TRUE; } else if (GetLastError () == ERROR_BROKEN_PIPE) ; else { /* It was the write-end of the pipe. Check if it is writable. If NtQueryInformationFile fails, optimistically assume the pipe is writable. This could happen on Windows 9x, where NtQueryInformationFile is not available, or if we inherit a pipe that doesn't permit FILE_READ_ATTRIBUTES access on the write end (I think this should not happen since Windows XP SP2; WINE seems fine too). Otherwise, ensure that enough space is available for atomic writes. */ memset (&iosb, 0, sizeof (iosb)); memset (&fpli, 0, sizeof (fpli)); if (!NtQueryInformationFile || NtQueryInformationFile (h, &iosb, &fpli, sizeof (fpli), FilePipeLocalInformation) || fpli.WriteQuotaAvailable >= PIPE_BUF || (fpli.OutboundQuota < PIPE_BUF && fpli.WriteQuotaAvailable == fpli.OutboundQuota)) write = TRUE; } break; case FILE_TYPE_CHAR: write = TRUE; if (!(rbits->in[fd / CHAR_BIT] & (1 << (fd & (CHAR_BIT - 1))))) break; ret = WaitForSingleObject (h, 0); if (ret == WAIT_OBJECT_0) { if (!IsConsoleHandle (h)) { read = TRUE; break; } nbuffer = avail = 0; bRet = GetNumberOfConsoleInputEvents (h, &nbuffer); /* Screen buffers handles are filtered earlier. */ assert (bRet); if (nbuffer == 0) { except = TRUE; break; } irbuffer = (INPUT_RECORD *) alloca (nbuffer * sizeof (INPUT_RECORD)); bRet = PeekConsoleInput (h, irbuffer, nbuffer, &avail); if (!bRet || avail == 0) { except = TRUE; break; } for (i = 0; i < avail; i++) if (irbuffer[i].EventType == KEY_EVENT) read = TRUE; } break; default: ret = WaitForSingleObject (h, 0); write = TRUE; if (ret == WAIT_OBJECT_0) read = TRUE; break; } ret = 0; if (read && (rbits->in[fd / CHAR_BIT] & (1 << (fd & (CHAR_BIT - 1))))) { rbits->out[fd / CHAR_BIT] |= (1 << (fd & (CHAR_BIT - 1))); ret++; } if (write && (wbits->in[fd / CHAR_BIT] & (1 << (fd & (CHAR_BIT - 1))))) { wbits->out[fd / CHAR_BIT] |= (1 << (fd & (CHAR_BIT - 1))); ret++; } if (except && (xbits->in[fd / CHAR_BIT] & (1 << (fd & (CHAR_BIT - 1))))) { xbits->out[fd / CHAR_BIT] |= (1 << (fd & (CHAR_BIT - 1))); ret++; } return ret; } int rpl_select (int nfds, fd_set *rfds, fd_set *wfds, fd_set *xfds, struct timeval *timeout) #undef timeval { static struct timeval tv0; static HANDLE hEvent; HANDLE h, handle_array[FD_SETSIZE + 2]; fd_set handle_rfds, handle_wfds, handle_xfds; struct bitset rbits, wbits, xbits; unsigned char anyfds_in[FD_SETSIZE / CHAR_BIT]; DWORD ret, wait_timeout, nhandles, nsock, nbuffer; MSG msg; int i, fd, rc; clock_t tend; if (nfds > FD_SETSIZE) nfds = FD_SETSIZE; if (!timeout) wait_timeout = INFINITE; else { wait_timeout = timeout->tv_sec * 1000 + timeout->tv_usec / 1000; /* select is also used as a portable usleep. */ if (!rfds && !wfds && !xfds) { Sleep (wait_timeout); return 0; } } if (!hEvent) hEvent = CreateEvent (NULL, FALSE, FALSE, NULL); handle_array[0] = hEvent; nhandles = 1; nsock = 0; /* Copy descriptors to bitsets. At the same time, eliminate bits in the "wrong" direction for console input buffers and screen buffers, because screen buffers are waitable and they will block until a character is available. */ memset (&rbits, 0, sizeof (rbits)); memset (&wbits, 0, sizeof (wbits)); memset (&xbits, 0, sizeof (xbits)); memset (anyfds_in, 0, sizeof (anyfds_in)); if (rfds) for (i = 0; i < rfds->fd_count; i++) { fd = rfds->fd_array[i]; h = (HANDLE) _get_osfhandle (fd); if (IsConsoleHandle (h) && !GetNumberOfConsoleInputEvents (h, &nbuffer)) continue; rbits.in[fd / CHAR_BIT] |= 1 << (fd & (CHAR_BIT - 1)); anyfds_in[fd / CHAR_BIT] |= 1 << (fd & (CHAR_BIT - 1)); } else rfds = (fd_set *) alloca (sizeof (fd_set)); if (wfds) for (i = 0; i < wfds->fd_count; i++) { fd = wfds->fd_array[i]; h = (HANDLE) _get_osfhandle (fd); if (IsConsoleHandle (h) && GetNumberOfConsoleInputEvents (h, &nbuffer)) continue; wbits.in[fd / CHAR_BIT] |= 1 << (fd & (CHAR_BIT - 1)); anyfds_in[fd / CHAR_BIT] |= 1 << (fd & (CHAR_BIT - 1)); } else wfds = (fd_set *) alloca (sizeof (fd_set)); if (xfds) for (i = 0; i < xfds->fd_count; i++) { fd = xfds->fd_array[i]; xbits.in[fd / CHAR_BIT] |= 1 << (fd & (CHAR_BIT - 1)); anyfds_in[fd / CHAR_BIT] |= 1 << (fd & (CHAR_BIT - 1)); } else xfds = (fd_set *) alloca (sizeof (fd_set)); /* Zero all the fd_sets, including the application's. */ FD_ZERO (rfds); FD_ZERO (wfds); FD_ZERO (xfds); FD_ZERO (&handle_rfds); FD_ZERO (&handle_wfds); FD_ZERO (&handle_xfds); /* Classify handles. Create fd sets for sockets, poll the others. */ for (i = 0; i < nfds; i++) { if ((anyfds_in[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) == 0) continue; h = (HANDLE) _get_osfhandle (i); if (!h) { errno = EBADF; return -1; } if (IsSocketHandle (h)) { int requested = FD_CLOSE; /* See above; socket handles are mapped onto select, but we need to map descriptors to handles. */ if (rbits.in[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) { requested |= FD_READ | FD_ACCEPT; FD_SET ((SOCKET) h, rfds); FD_SET ((SOCKET) h, &handle_rfds); } if (wbits.in[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) { requested |= FD_WRITE | FD_CONNECT; FD_SET ((SOCKET) h, wfds); FD_SET ((SOCKET) h, &handle_wfds); } if (xbits.in[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) { requested |= FD_OOB; FD_SET ((SOCKET) h, xfds); FD_SET ((SOCKET) h, &handle_xfds); } WSAEventSelect ((SOCKET) h, hEvent, requested); nsock++; } else { handle_array[nhandles++] = h; /* Poll now. If we get an event, do not wait below. */ if (wait_timeout != 0 && windows_poll_handle (h, i, &rbits, &wbits, &xbits)) wait_timeout = 0; } } /* Place a sentinel at the end of the array. */ handle_array[nhandles] = NULL; /* When will the waiting period expire? */ if (wait_timeout != INFINITE) tend = clock () + wait_timeout; restart: if (wait_timeout == 0 || nsock == 0) rc = 0; else { /* See if we need to wait in the loop below. If any select is ready, do MsgWaitForMultipleObjects anyway to dispatch messages, but no need to call select again. */ rc = select (0, &handle_rfds, &handle_wfds, &handle_xfds, &tv0); if (rc == 0) { /* Restore the fd_sets for the other select we do below. */ memcpy (&handle_rfds, rfds, sizeof (fd_set)); memcpy (&handle_wfds, wfds, sizeof (fd_set)); memcpy (&handle_xfds, xfds, sizeof (fd_set)); } else wait_timeout = 0; } /* How much is left to wait? */ if (wait_timeout != INFINITE) { clock_t tnow = clock (); if (tend >= tnow) wait_timeout = tend - tnow; else wait_timeout = 0; } for (;;) { ret = MsgWaitForMultipleObjects (nhandles, handle_array, FALSE, wait_timeout, QS_ALLINPUT); if (ret == WAIT_OBJECT_0 + nhandles) { /* new input of some other kind */ BOOL bRet; while ((bRet = PeekMessage (&msg, NULL, 0, 0, PM_REMOVE)) != 0) { TranslateMessage (&msg); DispatchMessage (&msg); } } else break; } /* If we haven't done it yet, check the status of the sockets. */ if (rc == 0 && nsock > 0) rc = select (0, &handle_rfds, &handle_wfds, &handle_xfds, &tv0); if (nhandles > 1) { /* Count results that are not counted in the return value of select. */ nhandles = 1; for (i = 0; i < nfds; i++) { if ((anyfds_in[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) == 0) continue; h = (HANDLE) _get_osfhandle (i); if (h == handle_array[nhandles]) { /* Not a socket. */ nhandles++; windows_poll_handle (h, i, &rbits, &wbits, &xbits); if (rbits.out[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1))) || wbits.out[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1))) || xbits.out[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) rc++; } } if (rc == 0 && (wait_timeout == INFINITE /* If NHANDLES > 1, but no bits are set, it means we've been told incorrectly that some handle was signaled. This happens with anonymous pipes, which always cause MsgWaitForMultipleObjects to exit immediately, but no data is found ready to be read by windows_poll_handle. To avoid a total failure (whereby we return zero and don't wait at all), let's poll in a more busy loop. */ || (wait_timeout != 0 && nhandles > 1))) { /* Sleep 1 millisecond to avoid busy wait and retry with the original fd_sets. */ memcpy (&handle_rfds, rfds, sizeof (fd_set)); memcpy (&handle_wfds, wfds, sizeof (fd_set)); memcpy (&handle_xfds, xfds, sizeof (fd_set)); SleepEx (1, TRUE); goto restart; } if (timeout && wait_timeout == 0 && rc == 0) timeout->tv_sec = timeout->tv_usec = 0; } /* Now fill in the results. */ FD_ZERO (rfds); FD_ZERO (wfds); FD_ZERO (xfds); nhandles = 1; for (i = 0; i < nfds; i++) { if ((anyfds_in[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) == 0) continue; h = (HANDLE) _get_osfhandle (i); if (h != handle_array[nhandles]) { /* Perform handle->descriptor mapping. */ WSAEventSelect ((SOCKET) h, NULL, 0); if (FD_ISSET (h, &handle_rfds)) FD_SET (i, rfds); if (FD_ISSET (h, &handle_wfds)) FD_SET (i, wfds); if (FD_ISSET (h, &handle_xfds)) FD_SET (i, xfds); } else { /* Not a socket. */ nhandles++; if (rbits.out[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) FD_SET (i, rfds); if (wbits.out[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) FD_SET (i, wfds); if (xbits.out[i / CHAR_BIT] & (1 << (i & (CHAR_BIT - 1)))) FD_SET (i, xfds); } } return rc; } #else /* ! Native Windows. */ #include #include /* NULL */ #include #include #undef select int rpl_select (int nfds, fd_set *rfds, fd_set *wfds, fd_set *xfds, struct timeval *timeout) { int i; /* FreeBSD 8.2 has a bug: it does not always detect invalid fds. */ if (nfds < 0 || nfds > FD_SETSIZE) { errno = EINVAL; return -1; } for (i = 0; i < nfds; i++) { if (((rfds && FD_ISSET (i, rfds)) || (wfds && FD_ISSET (i, wfds)) || (xfds && FD_ISSET (i, xfds))) && dup2 (i, i) != i) return -1; } /* Interix 3.5 has a bug: it does not support nfds == 0. */ if (nfds == 0) { nfds = 1; rfds = NULL; wfds = NULL; xfds = NULL; } return select (nfds, rfds, wfds, xfds, timeout); } #endif gnuastro-0.5/bootstrapped/tests/raise.c0000644000175000017500000000325613217200023015254 00000000000000/* Provide a non-threads replacement for the POSIX raise function. Copyright (C) 2002-2003, 2005-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Jim Meyering and Bruno Haible */ #include /* Specification. */ #include #if HAVE_RAISE /* Native Windows platform. */ # include # if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" # endif # undef raise # if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int raise_nothrow (int sig) { int result; TRY_MSVC_INVAL { result = raise (sig); } CATCH_MSVC_INVAL { result = -1; errno = EINVAL; } DONE_MSVC_INVAL; return result; } # else # define raise_nothrow raise # endif #else /* An old Unix platform. */ # include # define rpl_raise raise #endif int rpl_raise (int sig) { #if GNULIB_defined_signal_blocking && GNULIB_defined_SIGPIPE if (sig == SIGPIPE) return _gl_raise_SIGPIPE (); #endif #if HAVE_RAISE return raise_nothrow (sig); #else return kill (getpid (), sig); #endif } gnuastro-0.5/bootstrapped/tests/putenv.c0000644000175000017500000001176413217200023015475 00000000000000/* Copyright (C) 1991, 1994, 1997-1998, 2000, 2003-2017 Free Software Foundation, Inc. NOTE: The canonical source of this file is maintained with the GNU C Library. Bugs can be reported to bug-glibc@prep.ai.mit.edu. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include /* Include errno.h *after* sys/types.h to work around header problems on AIX 3.2.5. */ #include #ifndef __set_errno # define __set_errno(ev) ((errno) = (ev)) #endif #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include #endif #if _LIBC # if HAVE_GNU_LD # define environ __environ # else extern char **environ; # endif #endif #if _LIBC /* This lock protects against simultaneous modifications of 'environ'. */ # include __libc_lock_define_initialized (static, envlock) # define LOCK __libc_lock_lock (envlock) # define UNLOCK __libc_lock_unlock (envlock) #else # define LOCK # define UNLOCK #endif static int _unsetenv (const char *name) { size_t len; #if !HAVE_DECL__PUTENV char **ep; #endif if (name == NULL || *name == '\0' || strchr (name, '=') != NULL) { __set_errno (EINVAL); return -1; } len = strlen (name); #if HAVE_DECL__PUTENV { int putenv_result, putenv_errno; char *name_ = malloc (len + 2); memcpy (name_, name, len); name_[len] = '='; name_[len + 1] = 0; putenv_result = _putenv (name_); putenv_errno = errno; free (name_); __set_errno (putenv_errno); return putenv_result; } #else LOCK; ep = environ; while (*ep != NULL) if (!strncmp (*ep, name, len) && (*ep)[len] == '=') { /* Found it. Remove this pointer by moving later ones back. */ char **dp = ep; do dp[0] = dp[1]; while (*dp++); /* Continue the loop in case NAME appears again. */ } else ++ep; UNLOCK; return 0; #endif } /* Put STRING, which is of the form "NAME=VALUE", in the environment. If STRING contains no '=', then remove STRING from the environment. */ int putenv (char *string) { const char *name_end = strchr (string, '='); char **ep; if (name_end == NULL) { /* Remove the variable from the environment. */ return _unsetenv (string); } #if HAVE_DECL__PUTENV /* Rely on _putenv to allocate the new environment. If other parts of the application use _putenv, the !HAVE_DECL__PUTENV code would fight over who owns the environ vector, causing a crash. */ if (name_end[1]) return _putenv (string); else { /* _putenv ("NAME=") unsets NAME, so invoke _putenv ("NAME= ") to allocate the environ vector and then replace the new entry with "NAME=". */ int putenv_result, putenv_errno; char *name_x = malloc (name_end - string + sizeof "= "); if (!name_x) return -1; memcpy (name_x, string, name_end - string + 1); name_x[name_end - string + 1] = ' '; name_x[name_end - string + 2] = 0; putenv_result = _putenv (name_x); putenv_errno = errno; for (ep = environ; *ep; ep++) if (strcmp (*ep, name_x) == 0) { *ep = string; break; } # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ if (putenv_result == 0) { /* _putenv propagated "NAME= " into the subprocess environment; fix that by calling SetEnvironmentVariable directly. */ name_x[name_end - string] = 0; putenv_result = SetEnvironmentVariable (name_x, "") ? 0 : -1; putenv_errno = ENOMEM; /* ENOMEM is the only way to fail. */ } # endif free (name_x); __set_errno (putenv_errno); return putenv_result; } #else for (ep = environ; *ep; ep++) if (strncmp (*ep, string, name_end - string) == 0 && (*ep)[name_end - string] == '=') break; if (*ep) *ep = string; else { static char **last_environ = NULL; size_t size = ep - environ; char **new_environ = malloc ((size + 2) * sizeof *new_environ); if (! new_environ) return -1; new_environ[0] = string; memcpy (new_environ + 1, environ, (size + 1) * sizeof *new_environ); free (last_environ); last_environ = new_environ; environ = new_environ; } return 0; #endif } gnuastro-0.5/bootstrapped/tests/pthread_sigmask.c0000644000175000017500000000534013217200023017312 00000000000000/* POSIX compatible signal blocking for threads. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #if PTHREAD_SIGMASK_INEFFECTIVE # include #endif #if PTHREAD_SIGMASK_UNBLOCK_BUG # include #endif int pthread_sigmask (int how, const sigset_t *new_mask, sigset_t *old_mask) #undef pthread_sigmask { #if HAVE_PTHREAD_SIGMASK int ret; # if PTHREAD_SIGMASK_INEFFECTIVE sigset_t omask, omask_copy; sigset_t *old_mask_ptr = &omask; sigemptyset (&omask); /* Add a signal unlikely to be blocked, so that OMASK_COPY is unlikely to match the actual mask. */ sigaddset (&omask, SIGILL); memcpy (&omask_copy, &omask, sizeof omask); # else sigset_t *old_mask_ptr = old_mask; # endif ret = pthread_sigmask (how, new_mask, old_mask_ptr); # if PTHREAD_SIGMASK_INEFFECTIVE if (ret == 0) { /* Detect whether pthread_sigmask is currently ineffective. Don't cache the information: libpthread.so could be dynamically loaded after the program started and after pthread_sigmask was called for the first time. */ if (memcmp (&omask_copy, &omask, sizeof omask) == 0 && pthread_sigmask (1729, &omask_copy, NULL) == 0) { /* pthread_sigmask is currently ineffective. The program is not linked to -lpthread. So use sigprocmask instead. */ return (sigprocmask (how, new_mask, old_mask) < 0 ? errno : 0); } if (old_mask) memcpy (old_mask, &omask, sizeof omask); } # endif # if PTHREAD_SIGMASK_FAILS_WITH_ERRNO if (ret == -1) return errno; # endif # if PTHREAD_SIGMASK_UNBLOCK_BUG if (ret == 0 && new_mask != NULL && (how == SIG_UNBLOCK || how == SIG_SETMASK)) { /* Give the OS the opportunity to raise signals that were pending before the pthread_sigmask call and have now been unblocked. */ usleep (1); } # endif return ret; #else int ret = sigprocmask (how, new_mask, old_mask); return (ret < 0 ? errno : 0); #endif } gnuastro-0.5/bootstrapped/tests/pipe.c0000644000175000017500000000252413217200023015103 00000000000000/* Create a pipe. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Native Windows API. */ /* Get _pipe(). */ # include /* Get _O_BINARY. */ # include int pipe (int fd[2]) { /* Mingw changes fd to {-1,-1} on failure, but this violates http://austingroupbugs.net/view.php?id=467 */ int tmp[2]; int result = _pipe (tmp, 4096, _O_BINARY); if (!result) { fd[0] = tmp[0]; fd[1] = tmp[1]; } return result; } #else # error "This platform lacks a pipe function, and Gnulib doesn't provide a replacement. This is a bug in Gnulib." #endif gnuastro-0.5/bootstrapped/tests/perror.c0000644000175000017500000000276413217200023015465 00000000000000/* Print a message describing error code. Copyright (C) 2008-2017 Free Software Foundation, Inc. Written by Bruno Haible and Simon Josefsson. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include #include "strerror-override.h" /* Use the system functions, not the gnulib overrides in this file. */ #undef fprintf void perror (const char *string) { char stackbuf[STACKBUF_LEN]; int ret; /* Our implementation guarantees that this will be a non-empty string, even if it returns EINVAL; and stackbuf should be sized large enough to avoid ERANGE. */ ret = strerror_r (errno, stackbuf, sizeof stackbuf); if (ret == ERANGE) abort (); if (string != NULL && *string != '\0') fprintf (stderr, "%s: %s\n", string, stackbuf); else fprintf (stderr, "%s\n", stackbuf); } gnuastro-0.5/bootstrapped/tests/open.c0000644000175000017500000001507613217200023015115 00000000000000/* Open a descriptor to a file. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_open doesn't recurse to rpl_open. */ #define __need_system_fcntl_h #include /* Get the original definition of open. It might be defined as a macro. */ #include #include #undef __need_system_fcntl_h static int orig_open (const char *filename, int flags, mode_t mode) { return open (filename, flags, mode); } /* Specification. */ /* Write "fcntl.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ #include "fcntl.h" #include "cloexec.h" #include #include #include #include #include #include #ifndef REPLACE_OPEN_DIRECTORY # define REPLACE_OPEN_DIRECTORY 0 #endif int open (const char *filename, int flags, ...) { /* 0 = unknown, 1 = yes, -1 = no. */ #if GNULIB_defined_O_CLOEXEC int have_cloexec = -1; #else static int have_cloexec; #endif mode_t mode; int fd; mode = 0; if (flags & O_CREAT) { va_list arg; va_start (arg, flags); /* We have to use PROMOTED_MODE_T instead of mode_t, otherwise GCC 4 creates crashing code when 'mode_t' is smaller than 'int'. */ mode = va_arg (arg, PROMOTED_MODE_T); va_end (arg); } #if GNULIB_defined_O_NONBLOCK /* The only known platform that lacks O_NONBLOCK is mingw, but it also lacks named pipes and Unix sockets, which are the only two file types that require non-blocking handling in open(). Therefore, it is safe to ignore O_NONBLOCK here. It is handy that mingw also lacks openat(), so that is also covered here. */ flags &= ~O_NONBLOCK; #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ if (strcmp (filename, "/dev/null") == 0) filename = "NUL"; #endif #if OPEN_TRAILING_SLASH_BUG /* If the filename ends in a slash and one of O_CREAT, O_WRONLY, O_RDWR is specified, then fail. Rationale: POSIX says that "A pathname that contains at least one non-slash character and that ends with one or more trailing slashes shall be resolved as if a single dot character ( '.' ) were appended to the pathname." and "The special filename dot shall refer to the directory specified by its predecessor." If the named file already exists as a directory, then - if O_CREAT is specified, open() must fail because of the semantics of O_CREAT, - if O_WRONLY or O_RDWR is specified, open() must fail because POSIX says that it fails with errno = EISDIR in this case. If the named file does not exist or does not name a directory, then - if O_CREAT is specified, open() must fail since open() cannot create directories, - if O_WRONLY or O_RDWR is specified, open() must fail because the file does not contain a '.' directory. */ if (flags & (O_CREAT | O_WRONLY | O_RDWR)) { size_t len = strlen (filename); if (len > 0 && filename[len - 1] == '/') { errno = EISDIR; return -1; } } #endif fd = orig_open (filename, flags & ~(have_cloexec <= 0 ? O_CLOEXEC : 0), mode); if (flags & O_CLOEXEC) { if (! have_cloexec) { if (0 <= fd) have_cloexec = 1; else if (errno == EINVAL) { fd = orig_open (filename, flags & ~O_CLOEXEC, mode); have_cloexec = -1; } } if (have_cloexec < 0 && 0 <= fd) set_cloexec_flag (fd, true); } #if REPLACE_FCHDIR /* Implementing fchdir and fdopendir requires the ability to open a directory file descriptor. If open doesn't support that (as on mingw), we use a dummy file that behaves the same as directories on Linux (ie. always reports EOF on attempts to read()), and override fstat() in fchdir.c to hide the fact that we have a dummy. */ if (REPLACE_OPEN_DIRECTORY && fd < 0 && errno == EACCES && ((flags & O_ACCMODE) == O_RDONLY || (O_SEARCH != O_RDONLY && (flags & O_ACCMODE) == O_SEARCH))) { struct stat statbuf; if (stat (filename, &statbuf) == 0 && S_ISDIR (statbuf.st_mode)) { /* Maximum recursion depth of 1. */ fd = open ("/dev/null", flags, mode); if (0 <= fd) fd = _gl_register_fd (fd, filename); } else errno = EACCES; } #endif #if OPEN_TRAILING_SLASH_BUG /* If the filename ends in a slash and fd does not refer to a directory, then fail. Rationale: POSIX says that "A pathname that contains at least one non-slash character and that ends with one or more trailing slashes shall be resolved as if a single dot character ( '.' ) were appended to the pathname." and "The special filename dot shall refer to the directory specified by its predecessor." If the named file without the slash is not a directory, open() must fail with ENOTDIR. */ if (fd >= 0) { /* We know len is positive, since open did not fail with ENOENT. */ size_t len = strlen (filename); if (filename[len - 1] == '/') { struct stat statbuf; if (fstat (fd, &statbuf) >= 0 && !S_ISDIR (statbuf.st_mode)) { close (fd); errno = ENOTDIR; return -1; } } } #endif #if REPLACE_FCHDIR if (!REPLACE_OPEN_DIRECTORY && 0 <= fd) fd = _gl_register_fd (fd, filename); #endif return fd; } gnuastro-0.5/bootstrapped/tests/nanosleep.c0000644000175000017500000002000613217200023016125 00000000000000/* Provide a replacement for the POSIX nanosleep function. Copyright (C) 1999-2000, 2002, 2004-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Jim Meyering and Bruno Haible for the native Windows part */ #include #include #include "intprops.h" #include "sig-handler.h" #include "verify.h" #include #include #include #include #include #include #include #include enum { BILLION = 1000 * 1000 * 1000 }; #if HAVE_BUG_BIG_NANOSLEEP int nanosleep (const struct timespec *requested_delay, struct timespec *remaining_delay) # undef nanosleep { /* nanosleep mishandles large sleeps due to internal overflow problems. The worst known case of this is Linux 2.6.9 with glibc 2.3.4, which can't sleep more than 24.85 days (2^31 milliseconds). Similarly, cygwin 1.5.x, which can't sleep more than 49.7 days (2^32 milliseconds). Solve this by breaking the sleep up into smaller chunks. */ if (requested_delay->tv_nsec < 0 || BILLION <= requested_delay->tv_nsec) { errno = EINVAL; return -1; } { /* Verify that time_t is large enough. */ verify (TYPE_MAXIMUM (time_t) / 24 / 24 / 60 / 60); const time_t limit = 24 * 24 * 60 * 60; time_t seconds = requested_delay->tv_sec; struct timespec intermediate; intermediate.tv_nsec = requested_delay->tv_nsec; while (limit < seconds) { int result; intermediate.tv_sec = limit; result = nanosleep (&intermediate, remaining_delay); seconds -= limit; if (result) { if (remaining_delay) remaining_delay->tv_sec += seconds; return result; } intermediate.tv_nsec = 0; } intermediate.tv_sec = seconds; return nanosleep (&intermediate, remaining_delay); } } #elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Native Windows platforms. */ # define WIN32_LEAN_AND_MEAN # include /* The Windows API function Sleep() has a resolution of about 15 ms and takes at least 5 ms to execute. We use this function for longer time periods. Additionally, we use busy-looping over short time periods, to get a resolution of about 0.01 ms. In order to measure such short timespans, we use the QueryPerformanceCounter() function. */ int nanosleep (const struct timespec *requested_delay, struct timespec *remaining_delay) { static bool initialized; /* Number of performance counter increments per nanosecond, or zero if it could not be determined. */ static double ticks_per_nanosecond; if (requested_delay->tv_nsec < 0 || BILLION <= requested_delay->tv_nsec) { errno = EINVAL; return -1; } /* For requested delays of one second or more, 15ms resolution is sufficient. */ if (requested_delay->tv_sec == 0) { if (!initialized) { /* Initialize ticks_per_nanosecond. */ LARGE_INTEGER ticks_per_second; if (QueryPerformanceFrequency (&ticks_per_second)) ticks_per_nanosecond = (double) ticks_per_second.QuadPart / 1000000000.0; initialized = true; } if (ticks_per_nanosecond) { /* QueryPerformanceFrequency worked. We can use QueryPerformanceCounter. Use a combination of Sleep and busy-looping. */ /* Number of milliseconds to pass to the Sleep function. Since Sleep can take up to 8 ms less or 8 ms more than requested (or maybe more if the system is loaded), we subtract 10 ms. */ int sleep_millis = (int) requested_delay->tv_nsec / 1000000 - 10; /* Determine how many ticks to delay. */ LONGLONG wait_ticks = requested_delay->tv_nsec * ticks_per_nanosecond; /* Start. */ LARGE_INTEGER counter_before; if (QueryPerformanceCounter (&counter_before)) { /* Wait until the performance counter has reached this value. We don't need to worry about overflow, because the performance counter is reset at reboot, and with a frequency of 3.6E6 ticks per second 63 bits suffice for over 80000 years. */ LONGLONG wait_until = counter_before.QuadPart + wait_ticks; /* Use Sleep for the longest part. */ if (sleep_millis > 0) Sleep (sleep_millis); /* Busy-loop for the rest. */ for (;;) { LARGE_INTEGER counter_after; if (!QueryPerformanceCounter (&counter_after)) /* QueryPerformanceCounter failed, but succeeded earlier. Should not happen. */ break; if (counter_after.QuadPart >= wait_until) /* The requested time has elapsed. */ break; } goto done; } } } /* Implementation for long delays and as fallback. */ Sleep (requested_delay->tv_sec * 1000 + requested_delay->tv_nsec / 1000000); done: /* Sleep is not interruptible. So there is no remaining delay. */ if (remaining_delay != NULL) { remaining_delay->tv_sec = 0; remaining_delay->tv_nsec = 0; } return 0; } #else /* Unix platforms lacking nanosleep. */ /* Some systems (MSDOS) don't have SIGCONT. Using SIGTERM here turns the signal-handling code below into a no-op on such systems. */ # ifndef SIGCONT # define SIGCONT SIGTERM # endif static sig_atomic_t volatile suspended; /* Handle SIGCONT. */ static void sighandler (int sig) { suspended = 1; } /* Suspend execution for at least *TS_DELAY seconds. */ static int my_usleep (const struct timespec *ts_delay) { struct timeval tv_delay; tv_delay.tv_sec = ts_delay->tv_sec; tv_delay.tv_usec = (ts_delay->tv_nsec + 999) / 1000; if (tv_delay.tv_usec == 1000000) { if (tv_delay.tv_sec == TYPE_MAXIMUM (time_t)) tv_delay.tv_usec = 1000000 - 1; /* close enough */ else { tv_delay.tv_sec++; tv_delay.tv_usec = 0; } } return select (0, NULL, NULL, NULL, &tv_delay); } /* Suspend execution for at least *REQUESTED_DELAY seconds. The *REMAINING_DELAY part isn't implemented yet. */ int nanosleep (const struct timespec *requested_delay, struct timespec *remaining_delay) { static bool initialized; if (requested_delay->tv_nsec < 0 || BILLION <= requested_delay->tv_nsec) { errno = EINVAL; return -1; } /* set up sig handler */ if (! initialized) { struct sigaction oldact; sigaction (SIGCONT, NULL, &oldact); if (get_handler (&oldact) != SIG_IGN) { struct sigaction newact; newact.sa_handler = sighandler; sigemptyset (&newact.sa_mask); newact.sa_flags = 0; sigaction (SIGCONT, &newact, NULL); } initialized = true; } suspended = 0; if (my_usleep (requested_delay) == -1) { if (suspended) { /* Calculate time remaining. */ /* FIXME: the code in sleep doesn't use this, so there's no rush to implement it. */ errno = EINTR; } return -1; } /* FIXME: Restore sig handler? */ return 0; } #endif gnuastro-0.5/bootstrapped/tests/lstat.c0000644000175000017500000000712513217200023015277 00000000000000/* Work around a bug of lstat on some systems Copyright (C) 1997-2006, 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Jim Meyering */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_lstat doesn't recurse to rpl_lstat. */ #define __need_system_sys_stat_h #include #if !HAVE_LSTAT /* On systems that lack symlinks, our replacement already defined lstat as stat, so there is nothing further to do other than avoid an empty file. */ typedef int dummy; #else /* HAVE_LSTAT */ /* Get the original definition of lstat. It might be defined as a macro. */ # include # include # undef __need_system_sys_stat_h static int orig_lstat (const char *filename, struct stat *buf) { return lstat (filename, buf); } /* Specification. */ /* Write "sys/stat.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ # include "sys/stat.h" # include "stat-time.h" # include # include /* lstat works differently on Linux and Solaris systems. POSIX (see "pathname resolution" in the glossary) requires that programs like 'ls' take into consideration the fact that FILE has a trailing slash when FILE is a symbolic link. On Linux and Solaris 10 systems, the lstat function already has the desired semantics (in treating 'lstat ("symlink/", sbuf)' just like 'lstat ("symlink/.", sbuf)', but on Solaris 9 and earlier it does not. If FILE has a trailing slash and specifies a symbolic link, then use stat() to get more info on the referent of FILE. If the referent is a non-directory, then set errno to ENOTDIR and return -1. Otherwise, return stat's result. */ int rpl_lstat (const char *file, struct stat *sbuf) { int result = orig_lstat (file, sbuf); /* This replacement file can blindly check against '/' rather than using the ISSLASH macro, because all platforms with '\\' either lack symlinks (mingw) or have working lstat (cygwin) and thus do not compile this file. 0 len should have already been filtered out above, with a failure return of ENOENT. */ if (result == 0) { if (S_ISDIR (sbuf->st_mode) || file[strlen (file) - 1] != '/') result = stat_time_normalize (result, sbuf); else { /* At this point, a trailing slash is permitted only on symlink-to-dir; but it should have found information on the directory, not the symlink. Call 'stat' to get info about the link's referent. Our replacement stat guarantees valid results, even if the symlink is not pointing to a directory. */ if (!S_ISLNK (sbuf->st_mode)) { errno = ENOTDIR; return -1; } result = stat (file, sbuf); } } return result; } #endif /* HAVE_LSTAT */ gnuastro-0.5/bootstrapped/tests/localtime-buffer.c0000644000175000017500000000313413217200023017364 00000000000000/* Provide access to the last buffer returned by localtime() or gmtime(). Copyright (C) 2001-2003, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* written by Jim Meyering */ #include /* Specification. */ #include "localtime-buffer.h" #if GETTIMEOFDAY_CLOBBERS_LOCALTIME || TZSET_CLOBBERS_LOCALTIME static struct tm tm_zero_buffer; struct tm *localtime_buffer_addr = &tm_zero_buffer; /* This is a wrapper for localtime. On the first call, record the address of the static buffer that localtime uses for its result. */ struct tm * rpl_localtime (time_t const *timep) { struct tm *tm = localtime (timep); if (localtime_buffer_addr == &tm_zero_buffer) localtime_buffer_addr = tm; return tm; } /* Same as above, since gmtime and localtime use the same buffer. */ struct tm * rpl_gmtime (time_t const *timep) { struct tm *tm = gmtime (timep); if (localtime_buffer_addr == &tm_zero_buffer) localtime_buffer_addr = tm; return tm; } #endif gnuastro-0.5/bootstrapped/tests/listen.c0000644000175000017500000000234313217200023015443 00000000000000/* listen.c --- wrappers for Windows listen function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #define WIN32_LEAN_AND_MEAN /* Get winsock2.h. */ #include /* Get set_winsock_errno, FD_TO_SOCKET etc. */ #include "w32sock.h" #undef listen int rpl_listen (int fd, int backlog) { SOCKET sock = FD_TO_SOCKET (fd); if (sock == INVALID_SOCKET) { errno = EBADF; return -1; } else { int r = listen (sock, backlog); if (r < 0) set_winsock_errno (); return r; } } gnuastro-0.5/bootstrapped/tests/isnanl.c0000644000175000017500000000152613217200023015433 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #define USE_LONG_DOUBLE #include "isnan.c" gnuastro-0.5/bootstrapped/tests/isnanf.c0000644000175000017500000000152013217200023015417 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #define USE_FLOAT #include "isnan.c" gnuastro-0.5/bootstrapped/tests/isnand.c0000644000175000017500000000147013217200023015421 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include "isnan.c" gnuastro-0.5/bootstrapped/tests/isnan.c0000644000175000017500000001560613217200023015263 00000000000000/* Test for NaN that does not need libm. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include /* Specification. */ #ifdef USE_LONG_DOUBLE /* Specification found in math.h or isnanl-nolibm.h. */ extern int rpl_isnanl (long double x) _GL_ATTRIBUTE_CONST; #elif ! defined USE_FLOAT /* Specification found in math.h or isnand-nolibm.h. */ extern int rpl_isnand (double x); #else /* defined USE_FLOAT */ /* Specification found in math.h or isnanf-nolibm.h. */ extern int rpl_isnanf (float x); #endif #include #include #include "float+.h" #ifdef USE_LONG_DOUBLE # define FUNC rpl_isnanl # define DOUBLE long double # define MAX_EXP LDBL_MAX_EXP # define MIN_EXP LDBL_MIN_EXP # if defined LDBL_EXPBIT0_WORD && defined LDBL_EXPBIT0_BIT # define KNOWN_EXPBIT0_LOCATION # define EXPBIT0_WORD LDBL_EXPBIT0_WORD # define EXPBIT0_BIT LDBL_EXPBIT0_BIT # endif # define SIZE SIZEOF_LDBL # define L_(literal) literal##L #elif ! defined USE_FLOAT # define FUNC rpl_isnand # define DOUBLE double # define MAX_EXP DBL_MAX_EXP # define MIN_EXP DBL_MIN_EXP # if defined DBL_EXPBIT0_WORD && defined DBL_EXPBIT0_BIT # define KNOWN_EXPBIT0_LOCATION # define EXPBIT0_WORD DBL_EXPBIT0_WORD # define EXPBIT0_BIT DBL_EXPBIT0_BIT # endif # define SIZE SIZEOF_DBL # define L_(literal) literal #else /* defined USE_FLOAT */ # define FUNC rpl_isnanf # define DOUBLE float # define MAX_EXP FLT_MAX_EXP # define MIN_EXP FLT_MIN_EXP # if defined FLT_EXPBIT0_WORD && defined FLT_EXPBIT0_BIT # define KNOWN_EXPBIT0_LOCATION # define EXPBIT0_WORD FLT_EXPBIT0_WORD # define EXPBIT0_BIT FLT_EXPBIT0_BIT # endif # define SIZE SIZEOF_FLT # define L_(literal) literal##f #endif #define EXP_MASK ((MAX_EXP - MIN_EXP) | 7) #define NWORDS \ ((sizeof (DOUBLE) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { DOUBLE value; unsigned int word[NWORDS]; } memory_double; /* Most hosts nowadays use IEEE floating point, so they use IEC 60559 representations, have infinities and NaNs, and do not trap on exceptions. Define IEEE_FLOATING_POINT if this host is one of the typical ones. The C11 macro __STDC_IEC_559__ is close to what is wanted here, but is not quite right because this file does not require all the features of C11 Annex F (and does not require C11 at all, for that matter). */ #define IEEE_FLOATING_POINT (FLT_RADIX == 2 && FLT_MANT_DIG == 24 \ && FLT_MIN_EXP == -125 && FLT_MAX_EXP == 128) int FUNC (DOUBLE x) { #if defined KNOWN_EXPBIT0_LOCATION && IEEE_FLOATING_POINT # if defined USE_LONG_DOUBLE && ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Special CPU dependent code is needed to treat bit patterns outside the IEEE 754 specification (such as Pseudo-NaNs, Pseudo-Infinities, Pseudo-Zeroes, Unnormalized Numbers, and Pseudo-Denormals) as NaNs. These bit patterns are: - exponent = 0x0001..0x7FFF, mantissa bit 63 = 0, - exponent = 0x0000, mantissa bit 63 = 1. The NaN bit pattern is: - exponent = 0x7FFF, mantissa >= 0x8000000000000001. */ memory_double m; unsigned int exponent; m.value = x; exponent = (m.word[EXPBIT0_WORD] >> EXPBIT0_BIT) & EXP_MASK; # ifdef WORDS_BIGENDIAN /* Big endian: EXPBIT0_WORD = 0, EXPBIT0_BIT = 16. */ if (exponent == 0) return 1 & (m.word[0] >> 15); else if (exponent == EXP_MASK) return (((m.word[0] ^ 0x8000U) << 16) | m.word[1] | (m.word[2] >> 16)) != 0; else return 1 & ~(m.word[0] >> 15); # else /* Little endian: EXPBIT0_WORD = 2, EXPBIT0_BIT = 0. */ if (exponent == 0) return (m.word[1] >> 31); else if (exponent == EXP_MASK) return ((m.word[1] ^ 0x80000000U) | m.word[0]) != 0; else return (m.word[1] >> 31) ^ 1; # endif # else /* Be careful to not do any floating-point operation on x, such as x == x, because x may be a signaling NaN. */ # if defined __SUNPRO_C || defined __ICC || defined _MSC_VER \ || defined __DECC || defined __TINYC__ \ || (defined __sgi && !defined __GNUC__) /* The Sun C 5.0, Intel ICC 10.0, Microsoft Visual C/C++ 9.0, Compaq (ex-DEC) 6.4, and TinyCC compilers don't recognize the initializers as constant expressions. The Compaq compiler also fails when constant-folding 0.0 / 0.0 even when constant-folding is not required. The Microsoft Visual C/C++ compiler also fails when constant-folding 1.0 / 0.0 even when constant-folding is not required. The SGI MIPSpro C compiler complains about "floating-point operation result is out of range". */ static DOUBLE zero = L_(0.0); memory_double nan; DOUBLE plus_inf = L_(1.0) / zero; DOUBLE minus_inf = -L_(1.0) / zero; nan.value = zero / zero; # else static memory_double nan = { L_(0.0) / L_(0.0) }; static DOUBLE plus_inf = L_(1.0) / L_(0.0); static DOUBLE minus_inf = -L_(1.0) / L_(0.0); # endif { memory_double m; /* A NaN can be recognized through its exponent. But exclude +Infinity and -Infinity, which have the same exponent. */ m.value = x; if (((m.word[EXPBIT0_WORD] ^ nan.word[EXPBIT0_WORD]) & (EXP_MASK << EXPBIT0_BIT)) == 0) return (memcmp (&m.value, &plus_inf, SIZE) != 0 && memcmp (&m.value, &minus_inf, SIZE) != 0); else return 0; } # endif #else /* The configuration did not find sufficient information, or does not use IEEE floating point. Give up about the signaling NaNs; handle only the quiet NaNs. */ if (x == x) { # if defined USE_LONG_DOUBLE && ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Detect any special bit patterns that pass ==; see comment above. */ memory_double m1; memory_double m2; memset (&m1.value, 0, SIZE); memset (&m2.value, 0, SIZE); m1.value = x; m2.value = x + (x ? 0.0L : -0.0L); if (memcmp (&m1.value, &m2.value, SIZE) != 0) return 1; # endif return 0; } else return 1; #endif } gnuastro-0.5/bootstrapped/tests/isblank.c0000644000175000017500000000246713217200023015577 00000000000000/* Test whether a character is a blank. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include int isblank (int c) { /* On all known platforms, in all predefined locales, isblank(c) is likely equivalent with (c == ' ' || c == '\t'). Look at the glibc definition (in glibc/localedata/locales/i18n): The "blank" characters are '\t', ' ', U+1680, U+180E, U+2000..U+2006, U+2008..U+200A, U+205F, U+3000, and none except the first two is present in a common 8-bit encoding. Therefore the substitute for other platforms is not more complicated than this. */ return (c == ' ' || c == '\t'); } gnuastro-0.5/bootstrapped/tests/ioctl.c0000644000175000017500000000435313217200022015261 00000000000000/* ioctl.c --- wrappers for Windows ioctl function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #include #include #if HAVE_IOCTL /* Provide a wrapper with the POSIX prototype. */ # undef ioctl int rpl_ioctl (int fd, int request, ... /* {void *,char *} arg */) { void *buf; va_list args; va_start (args, request); buf = va_arg (args, void *); va_end (args); /* Cast 'request' so that when the system's ioctl function takes a 64-bit request argument, the value gets zero-extended, not sign-extended. */ return ioctl (fd, (unsigned int) request, buf); } #else /* mingw */ # include /* Get HANDLE. */ # define WIN32_LEAN_AND_MEAN # include # include "fd-hook.h" /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif static int primary_ioctl (int fd, int request, void *arg) { /* We don't support FIONBIO on pipes here. If you want to make pipe fds non-blocking, use the gnulib 'nonblocking' module, until gnulib implements fcntl F_GETFL / F_SETFL with O_NONBLOCK. */ if ((HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE) errno = ENOSYS; else errno = EBADF; return -1; } int ioctl (int fd, int request, ... /* {void *,char *} arg */) { void *arg; va_list args; va_start (args, request); arg = va_arg (args, void *); va_end (args); # if WINDOWS_SOCKETS return execute_all_ioctl_hooks (primary_ioctl, fd, request, arg); # else return primary_ioctl (fd, request, arg); # endif } #endif gnuastro-0.5/bootstrapped/tests/inet_pton.c0000644000175000017500000001537313217200022016152 00000000000000/* inet_pton.c -- convert IPv4 and IPv6 addresses from text to binary form Copyright (C) 2006, 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* * Copyright (c) 1996,1999 by Internet Software Consortium. * * Permission to use, copy, modify, and distribute this software for any * purpose with or without fee is hereby granted, provided that the above * copyright notice and this permission notice appear in all copies. * * THE SOFTWARE IS PROVIDED "AS IS" AND INTERNET SOFTWARE CONSORTIUM DISCLAIMS * ALL WARRANTIES WITH REGARD TO THIS SOFTWARE INCLUDING ALL IMPLIED WARRANTIES * OF MERCHANTABILITY AND FITNESS. IN NO EVENT SHALL INTERNET SOFTWARE * CONSORTIUM BE LIABLE FOR ANY SPECIAL, DIRECT, INDIRECT, OR CONSEQUENTIAL * DAMAGES OR ANY DAMAGES WHATSOEVER RESULTING FROM LOSS OF USE, DATA OR * PROFITS, WHETHER IN AN ACTION OF CONTRACT, NEGLIGENCE OR OTHER TORTIOUS * ACTION, ARISING OUT OF OR IN CONNECTION WITH THE USE OR PERFORMANCE OF THIS * SOFTWARE. */ #include /* Specification. */ #include #if HAVE_DECL_INET_PTON # undef inet_pton int rpl_inet_pton (int af, const char *restrict src, void *restrict dst) { return inet_pton (af, src, dst); } #else # include # include # include # define NS_INADDRSZ 4 # define NS_IN6ADDRSZ 16 # define NS_INT16SZ 2 /* * WARNING: Don't even consider trying to compile this on a system where * sizeof(int) < 4. sizeof(int) > 4 is fine; all the world's not a VAX. */ static int inet_pton4 (const char *src, unsigned char *dst); # if HAVE_IPV6 static int inet_pton6 (const char *src, unsigned char *dst); # endif /* int * inet_pton(af, src, dst) * convert from presentation format (which usually means ASCII printable) * to network format (which is usually some kind of binary format). * return: * 1 if the address was valid for the specified address family * 0 if the address wasn't valid ('dst' is untouched in this case) * -1 if some other error occurred ('dst' is untouched in this case, too) * author: * Paul Vixie, 1996. */ int inet_pton (int af, const char *restrict src, void *restrict dst) { switch (af) { case AF_INET: return (inet_pton4 (src, dst)); # if HAVE_IPV6 case AF_INET6: return (inet_pton6 (src, dst)); # endif default: errno = EAFNOSUPPORT; return (-1); } /* NOTREACHED */ } /* int * inet_pton4(src, dst) * like inet_aton() but without all the hexadecimal, octal (with the * exception of 0) and shorthand. * return: * 1 if 'src' is a valid dotted quad, else 0. * notice: * does not touch 'dst' unless it's returning 1. * author: * Paul Vixie, 1996. */ static int inet_pton4 (const char *restrict src, unsigned char *restrict dst) { int saw_digit, octets, ch; unsigned char tmp[NS_INADDRSZ], *tp; saw_digit = 0; octets = 0; *(tp = tmp) = 0; while ((ch = *src++) != '\0') { if (ch >= '0' && ch <= '9') { unsigned new = *tp * 10 + (ch - '0'); if (saw_digit && *tp == 0) return (0); if (new > 255) return (0); *tp = new; if (!saw_digit) { if (++octets > 4) return (0); saw_digit = 1; } } else if (ch == '.' && saw_digit) { if (octets == 4) return (0); *++tp = 0; saw_digit = 0; } else return (0); } if (octets < 4) return (0); memcpy (dst, tmp, NS_INADDRSZ); return (1); } # if HAVE_IPV6 /* int * inet_pton6(src, dst) * convert presentation level address to network order binary form. * return: * 1 if 'src' is a valid [RFC1884 2.2] address, else 0. * notice: * (1) does not touch 'dst' unless it's returning 1. * (2) :: in a full address is silently ignored. * credit: * inspired by Mark Andrews. * author: * Paul Vixie, 1996. */ static int inet_pton6 (const char *restrict src, unsigned char *restrict dst) { static const char xdigits[] = "0123456789abcdef"; unsigned char tmp[NS_IN6ADDRSZ], *tp, *endp, *colonp; const char *curtok; int ch, saw_xdigit; unsigned val; tp = memset (tmp, '\0', NS_IN6ADDRSZ); endp = tp + NS_IN6ADDRSZ; colonp = NULL; /* Leading :: requires some special handling. */ if (*src == ':') if (*++src != ':') return (0); curtok = src; saw_xdigit = 0; val = 0; while ((ch = c_tolower (*src++)) != '\0') { const char *pch; pch = strchr (xdigits, ch); if (pch != NULL) { val <<= 4; val |= (pch - xdigits); if (val > 0xffff) return (0); saw_xdigit = 1; continue; } if (ch == ':') { curtok = src; if (!saw_xdigit) { if (colonp) return (0); colonp = tp; continue; } else if (*src == '\0') { return (0); } if (tp + NS_INT16SZ > endp) return (0); *tp++ = (u_char) (val >> 8) & 0xff; *tp++ = (u_char) val & 0xff; saw_xdigit = 0; val = 0; continue; } if (ch == '.' && ((tp + NS_INADDRSZ) <= endp) && inet_pton4 (curtok, tp) > 0) { tp += NS_INADDRSZ; saw_xdigit = 0; break; /* '\0' was seen by inet_pton4(). */ } return (0); } if (saw_xdigit) { if (tp + NS_INT16SZ > endp) return (0); *tp++ = (u_char) (val >> 8) & 0xff; *tp++ = (u_char) val & 0xff; } if (colonp != NULL) { /* * Since some memmove()'s erroneously fail to handle * overlapping regions, we'll do the shift by hand. */ const int n = tp - colonp; int i; if (tp == endp) return (0); for (i = 1; i <= n; i++) { endp[-i] = colonp[n - i]; colonp[n - i] = 0; } tp = endp; } if (tp != endp) return (0); memcpy (dst, tmp, NS_IN6ADDRSZ); return (1); } # endif #endif gnuastro-0.5/bootstrapped/tests/gettimeofday.c0000644000175000017500000001073713217200022016633 00000000000000/* Provide gettimeofday for systems that don't have it or for which it's broken. Copyright (C) 2001-2003, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* written by Jim Meyering */ #include /* Specification. */ #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WINDOWS_NATIVE # include #endif #include "localtime-buffer.h" #ifdef WINDOWS_NATIVE /* GetSystemTimePreciseAsFileTime was introduced only in Windows 8. */ typedef void (WINAPI * GetSystemTimePreciseAsFileTimeFuncType) (FILETIME *lpTime); static GetSystemTimePreciseAsFileTimeFuncType GetSystemTimePreciseAsFileTimeFunc = NULL; static BOOL initialized = FALSE; static void initialize (void) { HMODULE kernel32 = LoadLibrary ("kernel32.dll"); if (kernel32 != NULL) { GetSystemTimePreciseAsFileTimeFunc = (GetSystemTimePreciseAsFileTimeFuncType) GetProcAddress (kernel32, "GetSystemTimePreciseAsFileTime"); } initialized = TRUE; } #endif /* This is a wrapper for gettimeofday. It is used only on systems that lack this function, or whose implementation of this function causes problems. Work around the bug in some systems whereby gettimeofday clobbers the static buffer that localtime uses for its return value. The gettimeofday function from Mac OS X 10.0.4 (i.e., Darwin 1.3.7) has this problem. */ int gettimeofday (struct timeval *restrict tv, void *restrict tz) { #undef gettimeofday #ifdef WINDOWS_NATIVE /* On native Windows, there are two ways to get the current time: GetSystemTimeAsFileTime or GetSystemTimePreciseAsFileTime . GetSystemTimeAsFileTime produces values that jump by increments of 15.627 milliseconds (!) on average. Whereas GetSystemTimePreciseAsFileTime values usually jump by 1 or 2 microseconds. More discussion on this topic: . */ FILETIME current_time; if (!initialized) initialize (); if (GetSystemTimePreciseAsFileTimeFunc != NULL) GetSystemTimePreciseAsFileTimeFunc (¤t_time); else GetSystemTimeAsFileTime (¤t_time); /* Convert from FILETIME to 'struct timeval'. */ /* FILETIME: */ ULONGLONG since_1601 = ((ULONGLONG) current_time.dwHighDateTime << 32) | (ULONGLONG) current_time.dwLowDateTime; /* Between 1601-01-01 and 1970-01-01 there were 280 normal years and 89 leap years, in total 134774 days. */ ULONGLONG since_1970 = since_1601 - (ULONGLONG) 134774 * (ULONGLONG) 86400 * (ULONGLONG) 10000000; ULONGLONG microseconds_since_1970 = since_1970 / (ULONGLONG) 10; tv->tv_sec = microseconds_since_1970 / (ULONGLONG) 1000000; tv->tv_usec = microseconds_since_1970 % (ULONGLONG) 1000000; return 0; #else # if HAVE_GETTIMEOFDAY # if GETTIMEOFDAY_CLOBBERS_LOCALTIME /* Save and restore the contents of the buffer used for localtime's result around the call to gettimeofday. */ struct tm save = *localtime_buffer_addr; # endif # if defined timeval /* 'struct timeval' overridden by gnulib? */ # undef timeval struct timeval otv; int result = gettimeofday (&otv, (struct timezone *) tz); if (result == 0) { tv->tv_sec = otv.tv_sec; tv->tv_usec = otv.tv_usec; } # else int result = gettimeofday (tv, (struct timezone *) tz); # endif # if GETTIMEOFDAY_CLOBBERS_LOCALTIME *localtime_buffer_addr = save; # endif return result; # else # if !defined OK_TO_USE_1S_CLOCK # error "Only 1-second nominal clock resolution found. Is that intended?" \ "If so, compile with the -DOK_TO_USE_1S_CLOCK option." # endif tv->tv_sec = time (NULL); tv->tv_usec = 0; return 0; # endif #endif } gnuastro-0.5/bootstrapped/tests/getpagesize.c0000644000175000017500000000227513217200022016457 00000000000000/* getpagesize emulation for systems where it cannot be done in a C macro. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible and Martin Lambers. */ #include /* Specification. */ #include /* This implementation is only for native Windows systems. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include int getpagesize (void) { SYSTEM_INFO system_info; GetSystemInfo (&system_info); return system_info.dwPageSize; } #endif gnuastro-0.5/bootstrapped/tests/getdtablesize.c0000644000175000017500000000657313217200022017003 00000000000000/* getdtablesize() function: Return maximum possible file descriptor value + 1. Copyright (C) 2008-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include # if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" # endif # if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int _setmaxstdio_nothrow (int newmax) { int result; TRY_MSVC_INVAL { result = _setmaxstdio (newmax); } CATCH_MSVC_INVAL { result = -1; } DONE_MSVC_INVAL; return result; } # else # define _setmaxstdio_nothrow _setmaxstdio # endif /* Cache for the previous getdtablesize () result. Safe to cache because Windows also lacks setrlimit. */ static int dtablesize; int getdtablesize (void) { if (dtablesize == 0) { /* We are looking for the number N such that the valid file descriptors are 0..N-1. It can be obtained through a loop as follows: { int fd; for (fd = 3; fd < 65536; fd++) if (dup2 (0, fd) == -1) break; return fd; } On Windows XP, the result is 2048. The drawback of this loop is that it allocates memory for a libc internal array that is never freed. The number N can also be obtained as the upper bound for _getmaxstdio (). _getmaxstdio () returns the maximum number of open FILE objects. The sanity check in _setmaxstdio reveals the maximum number of file descriptors. This too allocates memory, but it is freed when we call _setmaxstdio with the original value. */ int orig_max_stdio = _getmaxstdio (); unsigned int bound; for (bound = 0x10000; _setmaxstdio_nothrow (bound) < 0; bound = bound / 2) ; _setmaxstdio_nothrow (orig_max_stdio); dtablesize = bound; } return dtablesize; } #else # include # include # ifndef RLIM_SAVED_CUR # define RLIM_SAVED_CUR RLIM_INFINITY # endif # ifndef RLIM_SAVED_MAX # define RLIM_SAVED_MAX RLIM_INFINITY # endif # ifdef __CYGWIN__ /* Cygwin 1.7.25 auto-increases the RLIMIT_NOFILE soft limit until it hits the compile-time constant hard limit of 3200. We might as well just report the hard limit. */ # define rlim_cur rlim_max # endif int getdtablesize (void) { struct rlimit lim; if (getrlimit (RLIMIT_NOFILE, &lim) == 0 && 0 <= lim.rlim_cur && lim.rlim_cur <= INT_MAX && lim.rlim_cur != RLIM_INFINITY && lim.rlim_cur != RLIM_SAVED_CUR && lim.rlim_cur != RLIM_SAVED_MAX) return lim.rlim_cur; return INT_MAX; } #endif gnuastro-0.5/bootstrapped/tests/getcwd-lgpl.c0000644000175000017500000000606713217200022016364 00000000000000/* Copyright (C) 2011-2017 Free Software Foundation, Inc. This file is part of gnulib. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification */ #include #include #include #include #if GNULIB_GETCWD /* Favor GPL getcwd.c if both getcwd and getcwd-lgpl modules are in use. */ typedef int dummy; #else /* Get the name of the current working directory, and put it in SIZE bytes of BUF. Returns NULL if the directory couldn't be determined (perhaps because the absolute name was longer than PATH_MAX, or because of missing read/search permissions on parent directories) or SIZE was too small. If successful, returns BUF. If BUF is NULL, an array is allocated with 'malloc'; the array is SIZE bytes long, unless SIZE == 0, in which case it is as big as necessary. */ # undef getcwd char * rpl_getcwd (char *buf, size_t size) { char *ptr; char *result; /* Handle single size operations. */ if (buf) { if (!size) { errno = EINVAL; return NULL; } return getcwd (buf, size); } if (size) { buf = malloc (size); if (!buf) { errno = ENOMEM; return NULL; } result = getcwd (buf, size); if (!result) { int saved_errno = errno; free (buf); errno = saved_errno; } return result; } /* Flexible sizing requested. Avoid over-allocation for the common case of a name that fits within a 4k page, minus some space for local variables, to be sure we don't skip over a guard page. */ { char tmp[4032]; size = sizeof tmp; ptr = getcwd (tmp, size); if (ptr) { result = strdup (ptr); if (!result) errno = ENOMEM; return result; } if (errno != ERANGE) return NULL; } /* My what a large directory name we have. */ do { size <<= 1; ptr = realloc (buf, size); if (ptr == NULL) { free (buf); errno = ENOMEM; return NULL; } buf = ptr; result = getcwd (buf, size); } while (!result && errno == ERANGE); if (!result) { int saved_errno = errno; free (buf); errno = saved_errno; } else { /* Trim to fit, if possible. */ result = realloc (buf, strlen (buf) + 1); if (!result) result = buf; } return result; } #endif gnuastro-0.5/bootstrapped/tests/ftruncate.c0000644000175000017500000001161613217200022016142 00000000000000/* ftruncate emulations for native Windows. Copyright (C) 1992-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include #if HAVE_CHSIZE /* A native Windows platform. */ # include # if _GL_WINDOWS_64_BIT_OFF_T /* Large File Support: off_t is 64-bit, but chsize() takes only a 32-bit argument. So, define a 64-bit safe SetFileSize function ourselves. */ /* Ensure that declares GetFileSizeEx. */ # undef _WIN32_WINNT # define _WIN32_WINNT _WIN32_WINNT_WIN2K /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif static BOOL SetFileSize (HANDLE h, LONGLONG size) { LARGE_INTEGER old_size; if (!GetFileSizeEx (h, &old_size)) return FALSE; if (size != old_size.QuadPart) { /* Duplicate the handle, so we are free to modify its file position. */ HANDLE curr_process = GetCurrentProcess (); HANDLE tmph; if (!DuplicateHandle (curr_process, /* SourceProcessHandle */ h, /* SourceHandle */ curr_process, /* TargetProcessHandle */ (PHANDLE) &tmph, /* TargetHandle */ (DWORD) 0, /* DesiredAccess */ FALSE, /* InheritHandle */ DUPLICATE_SAME_ACCESS)) /* Options */ return FALSE; if (size < old_size.QuadPart) { /* Reduce the size. */ LONG size_hi = (LONG) (size >> 32); if (SetFilePointer (tmph, (LONG) size, &size_hi, FILE_BEGIN) == INVALID_SET_FILE_POINTER && GetLastError() != NO_ERROR) { CloseHandle (tmph); return FALSE; } if (!SetEndOfFile (tmph)) { CloseHandle (tmph); return FALSE; } } else { /* Increase the size by adding zero bytes at the end. */ static char zero_bytes[1024]; LONG pos_hi = 0; LONG pos_lo = SetFilePointer (tmph, (LONG) 0, &pos_hi, FILE_END); LONGLONG pos; if (pos_lo == INVALID_SET_FILE_POINTER && GetLastError() != NO_ERROR) { CloseHandle (tmph); return FALSE; } pos = ((LONGLONG) pos_hi << 32) | (ULONGLONG) (ULONG) pos_lo; while (pos < size) { DWORD written; LONGLONG count = size - pos; if (count > sizeof (zero_bytes)) count = sizeof (zero_bytes); if (!WriteFile (tmph, zero_bytes, (DWORD) count, &written, NULL) || written == 0) { CloseHandle (tmph); return FALSE; } pos += (ULONGLONG) (ULONG) written; } } /* Close the handle. */ CloseHandle (tmph); } return TRUE; } int ftruncate (int fd, off_t length) { HANDLE handle = (HANDLE) _get_osfhandle (fd); if (handle == INVALID_HANDLE_VALUE) { errno = EBADF; return -1; } if (length < 0) { errno = EINVAL; return -1; } if (!SetFileSize (handle, length)) { switch (GetLastError ()) { case ERROR_ACCESS_DENIED: errno = EACCES; break; case ERROR_HANDLE_DISK_FULL: case ERROR_DISK_FULL: case ERROR_DISK_TOO_FRAGMENTED: errno = ENOSPC; break; default: errno = EIO; break; } return -1; } return 0; } # else # include # if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" static int chsize_nothrow (int fd, long length) { int result; TRY_MSVC_INVAL { result = chsize (fd, length); } CATCH_MSVC_INVAL { result = -1; errno = EBADF; } DONE_MSVC_INVAL; return result; } # else # define chsize_nothrow chsize # endif int ftruncate (int fd, off_t length) { return chsize_nothrow (fd, length); } # endif #endif gnuastro-0.5/bootstrapped/tests/stat-w32.c0000644000175000017500000003736213217200023015542 00000000000000/* Core of implementation of fstat and stat for native Windows. Copyright (C) 2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible. */ #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Ensure that defines FILE_ID_INFO. */ #undef _WIN32_WINNT #define _WIN32_WINNT _WIN32_WINNT_WIN8 #include #include #include #include #include #include #include /* Specification. */ #include "stat-w32.h" #include "pathmax.h" #include "verify.h" #if _GL_WINDOWS_STAT_INODES == 2 /* GetFileInformationByHandleEx was introduced only in Windows Vista. */ typedef DWORD (WINAPI * GetFileInformationByHandleExFuncType) (HANDLE hFile, FILE_INFO_BY_HANDLE_CLASS fiClass, LPVOID lpBuffer, DWORD dwBufferSize); static GetFileInformationByHandleExFuncType GetFileInformationByHandleExFunc = NULL; #endif /* GetFinalPathNameByHandle was introduced only in Windows Vista. */ typedef DWORD (WINAPI * GetFinalPathNameByHandleFuncType) (HANDLE hFile, LPTSTR lpFilePath, DWORD lenFilePath, DWORD dwFlags); static GetFinalPathNameByHandleFuncType GetFinalPathNameByHandleFunc = NULL; static BOOL initialized = FALSE; static void initialize (void) { HMODULE kernel32 = LoadLibrary ("kernel32.dll"); if (kernel32 != NULL) { #if _GL_WINDOWS_STAT_INODES == 2 GetFileInformationByHandleExFunc = (GetFileInformationByHandleExFuncType) GetProcAddress (kernel32, "GetFileInformationByHandleEx"); #endif GetFinalPathNameByHandleFunc = (GetFinalPathNameByHandleFuncType) GetProcAddress (kernel32, "GetFinalPathNameByHandleA"); } initialized = TRUE; } /* Converts a FILETIME to GMT time since 1970-01-01 00:00:00. */ #if _GL_WINDOWS_STAT_TIMESPEC struct timespec _gl_convert_FILETIME_to_timespec (const FILETIME *ft) { struct timespec result; /* FILETIME: */ unsigned long long since_1601 = ((unsigned long long) ft->dwHighDateTime << 32) | (unsigned long long) ft->dwLowDateTime; if (since_1601 == 0) { result.tv_sec = 0; result.tv_nsec = 0; } else { /* Between 1601-01-01 and 1970-01-01 there were 280 normal years and 89 leap years, in total 134774 days. */ unsigned long long since_1970 = since_1601 - (unsigned long long) 134774 * (unsigned long long) 86400 * (unsigned long long) 10000000; result.tv_sec = since_1970 / (unsigned long long) 10000000; result.tv_nsec = (unsigned long) (since_1970 % (unsigned long long) 10000000) * 100; } return result; } #else time_t _gl_convert_FILETIME_to_POSIX (const FILETIME *ft) { /* FILETIME: */ unsigned long long since_1601 = ((unsigned long long) ft->dwHighDateTime << 32) | (unsigned long long) ft->dwLowDateTime; if (since_1601 == 0) return 0; else { /* Between 1601-01-01 and 1970-01-01 there were 280 normal years and 89 leap years, in total 134774 days. */ unsigned long long since_1970 = since_1601 - (unsigned long long) 134774 * (unsigned long long) 86400 * (unsigned long long) 10000000; return since_1970 / (unsigned long long) 10000000; } } #endif /* Fill *BUF with information about the file designated by H. PATH is the file name, if known, otherwise NULL. Return 0 if successful, or -1 with errno set upon failure. */ int _gl_fstat_by_handle (HANDLE h, const char *path, struct stat *buf) { /* GetFileType */ DWORD type = GetFileType (h); if (type == FILE_TYPE_DISK) { if (!initialized) initialize (); /* st_mode can be determined through GetFileAttributesEx or through GetFileInformationByHandle or through GetFileInformationByHandleEx with argument FileBasicInfo The latter requires -D_WIN32_WINNT=_WIN32_WINNT_VISTA or higher. */ BY_HANDLE_FILE_INFORMATION info; if (! GetFileInformationByHandle (h, &info)) goto failed; /* Test for error conditions before starting to fill *buf. */ if (sizeof (buf->st_size) <= 4 && info.nFileSizeHigh > 0) { errno = EOVERFLOW; return -1; } #if _GL_WINDOWS_STAT_INODES /* st_ino can be determined through GetFileInformationByHandle as 64 bits, or through GetFileInformationByHandleEx with argument FileIdInfo as 128 bits. The latter requires -D_WIN32_WINNT=_WIN32_WINNT_WIN8 or higher. */ /* Experiments show that GetFileInformationByHandleEx does not provide much more information than GetFileInformationByHandle: * The dwVolumeSerialNumber from GetFileInformationByHandle is equal to the low 32 bits of the 64-bit VolumeSerialNumber from GetFileInformationByHandleEx, and is apparently sufficient for identifying the device. * The nFileIndex from GetFileInformationByHandle is equal to the low 64 bits of the 128-bit FileId from GetFileInformationByHandleEx, and the high 64 bits of this 128-bit FileId are zero. * On a FAT file system, GetFileInformationByHandleEx fails with error ERROR_INVALID_PARAMETER, whereas GetFileInformationByHandle succeeds. * On a CIFS/SMB file system, GetFileInformationByHandleEx fails with error ERROR_INVALID_LEVEL, whereas GetFileInformationByHandle succeeds. */ # if _GL_WINDOWS_STAT_INODES == 2 if (GetFileInformationByHandleExFunc != NULL) { FILE_ID_INFO id; if (GetFileInformationByHandleExFunc (h, FileIdInfo, &id, sizeof (id))) { buf->st_dev = id.VolumeSerialNumber; verify (sizeof (ino_t) == sizeof (id.FileId)); memcpy (&buf->st_ino, &id.FileId, sizeof (ino_t)); goto ino_done; } else { switch (GetLastError ()) { case ERROR_INVALID_PARAMETER: /* older Windows version, or FAT */ case ERROR_INVALID_LEVEL: /* CIFS/SMB file system */ goto fallback; default: goto failed; } } } fallback: ; /* Fallback for older Windows versions. */ buf->st_dev = info.dwVolumeSerialNumber; buf->st_ino._gl_ino[0] = ((ULONGLONG) info.nFileIndexHigh << 32) | (ULONGLONG) info.nFileIndexLow; buf->st_ino._gl_ino[1] = 0; ino_done: ; # else /* _GL_WINDOWS_STAT_INODES == 1 */ buf->st_dev = info.dwVolumeSerialNumber; buf->st_ino = ((ULONGLONG) info.nFileIndexHigh << 32) | (ULONGLONG) info.nFileIndexLow; # endif #else /* st_ino is not wide enough for identifying a file on a device. Without st_ino, st_dev is pointless. */ buf->st_dev = 0; buf->st_ino = 0; #endif /* st_mode. */ unsigned int mode = /* XXX How to handle FILE_ATTRIBUTE_REPARSE_POINT ? */ ((info.dwFileAttributes & FILE_ATTRIBUTE_DIRECTORY) ? _S_IFDIR | S_IEXEC_UGO : _S_IFREG) | S_IREAD_UGO | ((info.dwFileAttributes & FILE_ATTRIBUTE_READONLY) ? 0 : S_IWRITE_UGO); if (!(info.dwFileAttributes & FILE_ATTRIBUTE_DIRECTORY)) { /* Determine whether the file is executable by looking at the file name suffix. If the file name is already known, use it. Otherwise, for non-empty files, it can be determined through GetFinalPathNameByHandle or through GetFileInformationByHandleEx with argument FileNameInfo Both require -D_WIN32_WINNT=_WIN32_WINNT_VISTA or higher. */ if (info.nFileSizeHigh > 0 || info.nFileSizeLow > 0) { char fpath[PATH_MAX]; if (path != NULL || (GetFinalPathNameByHandleFunc != NULL && GetFinalPathNameByHandleFunc (h, fpath, sizeof (fpath), VOLUME_NAME_NONE) < sizeof (fpath) && (path = fpath, 1))) { const char *last_dot = NULL; const char *p; for (p = path; *p != '\0'; p++) if (*p == '.') last_dot = p; if (last_dot != NULL) { const char *suffix = last_dot + 1; if (_stricmp (suffix, "exe") == 0 || _stricmp (suffix, "bat") == 0 || _stricmp (suffix, "cmd") == 0 || _stricmp (suffix, "com") == 0) mode |= S_IEXEC_UGO; } } else /* Cannot determine file name. Pretend that it is executable. */ mode |= S_IEXEC_UGO; } } buf->st_mode = mode; /* st_nlink can be determined through GetFileInformationByHandle or through GetFileInformationByHandleEx with argument FileStandardInfo The latter requires -D_WIN32_WINNT=_WIN32_WINNT_VISTA or higher. */ buf->st_nlink = (info.nNumberOfLinks > SHRT_MAX ? SHRT_MAX : info.nNumberOfLinks); /* There's no easy way to map the Windows SID concept to an integer. */ buf->st_uid = 0; buf->st_gid = 0; /* st_rdev is irrelevant for normal files and directories. */ buf->st_rdev = 0; /* st_size can be determined through GetFileSizeEx or through GetFileAttributesEx or through GetFileInformationByHandle or through GetFileInformationByHandleEx with argument FileStandardInfo The latter requires -D_WIN32_WINNT=_WIN32_WINNT_VISTA or higher. */ if (sizeof (buf->st_size) <= 4) /* Range check already done above. */ buf->st_size = info.nFileSizeLow; else buf->st_size = ((long long) info.nFileSizeHigh << 32) | (long long) info.nFileSizeLow; /* st_atime, st_mtime, st_ctime can be determined through GetFileTime or through GetFileAttributesEx or through GetFileInformationByHandle or through GetFileInformationByHandleEx with argument FileBasicInfo The latter requires -D_WIN32_WINNT=_WIN32_WINNT_VISTA or higher. */ #if _GL_WINDOWS_STAT_TIMESPEC buf->st_atim = _gl_convert_FILETIME_to_timespec (&info.ftLastAccessTime); buf->st_mtim = _gl_convert_FILETIME_to_timespec (&info.ftLastWriteTime); buf->st_ctim = _gl_convert_FILETIME_to_timespec (&info.ftCreationTime); #else buf->st_atime = _gl_convert_FILETIME_to_POSIX (&info.ftLastAccessTime); buf->st_mtime = _gl_convert_FILETIME_to_POSIX (&info.ftLastWriteTime); buf->st_ctime = _gl_convert_FILETIME_to_POSIX (&info.ftCreationTime); #endif return 0; } else if (type == FILE_TYPE_CHAR || type == FILE_TYPE_PIPE) { buf->st_dev = 0; #if _GL_WINDOWS_STAT_INODES == 2 buf->st_ino._gl_ino[0] = buf->st_ino._gl_ino[1] = 0; #else buf->st_ino = 0; #endif buf->st_mode = (type == FILE_TYPE_PIPE ? _S_IFIFO : _S_IFCHR); buf->st_nlink = 1; buf->st_uid = 0; buf->st_gid = 0; buf->st_rdev = 0; if (type == FILE_TYPE_PIPE) { /* PeekNamedPipe */ DWORD bytes_available; if (PeekNamedPipe (h, NULL, 0, NULL, &bytes_available, NULL)) buf->st_size = bytes_available; else buf->st_size = 0; } else buf->st_size = 0; #if _GL_WINDOWS_STAT_TIMESPEC buf->st_atim.tv_sec = 0; buf->st_atim.tv_nsec = 0; buf->st_mtim.tv_sec = 0; buf->st_mtim.tv_nsec = 0; buf->st_ctim.tv_sec = 0; buf->st_ctim.tv_nsec = 0; #else buf->st_atime = 0; buf->st_mtime = 0; buf->st_ctime = 0; #endif return 0; } else { errno = ENOENT; return -1; } failed: { DWORD error = GetLastError (); #if 0 fprintf (stderr, "_gl_fstat_by_handle error 0x%x\n", (unsigned int) error); #endif switch (error) { case ERROR_ACCESS_DENIED: case ERROR_SHARING_VIOLATION: errno = EACCES; break; case ERROR_OUTOFMEMORY: errno = ENOMEM; break; case ERROR_WRITE_FAULT: case ERROR_READ_FAULT: case ERROR_GEN_FAILURE: errno = EIO; break; default: errno = EINVAL; break; } return -1; } } #else /* This declaration is solely to ensure that after preprocessing this file is never empty. */ typedef int dummy; #endif gnuastro-0.5/bootstrapped/tests/fstat.c0000644000175000017500000000507513217200022015272 00000000000000/* fstat() replacement. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* If the user's config.h happens to include , let it include only the system's here, so that orig_fstat doesn't recurse to rpl_fstat. */ #define __need_system_sys_stat_h #include /* Get the original definition of fstat. It might be defined as a macro. */ #include #include #undef __need_system_sys_stat_h #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WINDOWS_NATIVE #endif #if !defined WINDOWS_NATIVE static int orig_fstat (int fd, struct stat *buf) { return fstat (fd, buf); } #endif /* Specification. */ /* Write "sys/stat.h" here, not , otherwise OSF/1 5.1 DTK cc eliminates this include because of the preliminary #include above. */ #include "sys/stat.h" #include "stat-time.h" #include #include #ifdef WINDOWS_NATIVE # define WIN32_LEAN_AND_MEAN # include # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif # include "stat-w32.h" #endif int rpl_fstat (int fd, struct stat *buf) { #if REPLACE_FCHDIR && REPLACE_OPEN_DIRECTORY /* Handle the case when rpl_open() used a dummy file descriptor to work around an open() that can't normally visit directories. */ const char *name = _gl_directory_name (fd); if (name != NULL) return stat (name, buf); #endif #ifdef WINDOWS_NATIVE /* Fill the fields ourselves, because the original fstat function returns values for st_atime, st_mtime, st_ctime that depend on the current time zone. See */ HANDLE h = (HANDLE) _get_osfhandle (fd); if (h == INVALID_HANDLE_VALUE) { errno = EBADF; return -1; } return _gl_fstat_by_handle (h, NULL, buf); #else return stat_time_normalize (orig_fstat (fd, buf), buf); #endif } gnuastro-0.5/bootstrapped/tests/fdopen.c0000644000175000017500000000273013217200022015417 00000000000000/* Open a stream with a given file descriptor. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #undef fdopen #if HAVE_MSVC_INVALID_PARAMETER_HANDLER static FILE * fdopen_nothrow (int fd, const char *mode) { FILE *result; TRY_MSVC_INVAL { result = fdopen (fd, mode); } CATCH_MSVC_INVAL { result = NULL; } DONE_MSVC_INVAL; return result; } #else # define fdopen_nothrow fdopen #endif FILE * rpl_fdopen (int fd, const char *mode) { int saved_errno = errno; FILE *fp; errno = 0; fp = fdopen_nothrow (fd, mode); if (fp == NULL) { if (errno == 0) errno = EBADF; } else errno = saved_errno; return fp; } gnuastro-0.5/bootstrapped/tests/fcntl.c0000644000175000017500000002733713217200022015264 00000000000000/* Provide file descriptor control. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Eric Blake . */ #include /* Specification. */ #include #include #include #include #include #if !HAVE_FCNTL # define rpl_fcntl fcntl #endif #undef fcntl #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif /* Upper bound on getdtablesize(). See lib/getdtablesize.c. */ # define OPEN_MAX_MAX 0x10000 /* Duplicate OLDFD into the first available slot of at least NEWFD, which must be positive, with FLAGS determining whether the duplicate will be inheritable. */ static int dupfd (int oldfd, int newfd, int flags) { /* Mingw has no way to create an arbitrary fd. Iterate until all file descriptors less than newfd are filled up. */ HANDLE curr_process = GetCurrentProcess (); HANDLE old_handle = (HANDLE) _get_osfhandle (oldfd); unsigned char fds_to_close[OPEN_MAX_MAX / CHAR_BIT]; unsigned int fds_to_close_bound = 0; int result; BOOL inherit = flags & O_CLOEXEC ? FALSE : TRUE; int mode; if (newfd < 0 || getdtablesize () <= newfd) { errno = EINVAL; return -1; } if (old_handle == INVALID_HANDLE_VALUE || (mode = setmode (oldfd, O_BINARY)) == -1) { /* oldfd is not open, or is an unassigned standard file descriptor. */ errno = EBADF; return -1; } setmode (oldfd, mode); flags |= mode; for (;;) { HANDLE new_handle; int duplicated_fd; unsigned int index; if (!DuplicateHandle (curr_process, /* SourceProcessHandle */ old_handle, /* SourceHandle */ curr_process, /* TargetProcessHandle */ (PHANDLE) &new_handle, /* TargetHandle */ (DWORD) 0, /* DesiredAccess */ inherit, /* InheritHandle */ DUPLICATE_SAME_ACCESS)) /* Options */ { switch (GetLastError ()) { case ERROR_TOO_MANY_OPEN_FILES: errno = EMFILE; break; case ERROR_INVALID_HANDLE: case ERROR_INVALID_TARGET_HANDLE: case ERROR_DIRECT_ACCESS_HANDLE: errno = EBADF; break; case ERROR_INVALID_PARAMETER: case ERROR_INVALID_FUNCTION: case ERROR_INVALID_ACCESS: errno = EINVAL; break; default: errno = EACCES; break; } result = -1; break; } duplicated_fd = _open_osfhandle ((intptr_t) new_handle, flags); if (duplicated_fd < 0) { CloseHandle (new_handle); result = -1; break; } if (newfd <= duplicated_fd) { result = duplicated_fd; break; } /* Set the bit duplicated_fd in fds_to_close[]. */ index = (unsigned int) duplicated_fd / CHAR_BIT; if (fds_to_close_bound <= index) { if (sizeof fds_to_close <= index) /* Need to increase OPEN_MAX_MAX. */ abort (); memset (fds_to_close + fds_to_close_bound, '\0', index + 1 - fds_to_close_bound); fds_to_close_bound = index + 1; } fds_to_close[index] |= 1 << ((unsigned int) duplicated_fd % CHAR_BIT); } /* Close the previous fds that turned out to be too small. */ { int saved_errno = errno; unsigned int duplicated_fd; for (duplicated_fd = 0; duplicated_fd < fds_to_close_bound * CHAR_BIT; duplicated_fd++) if ((fds_to_close[duplicated_fd / CHAR_BIT] >> (duplicated_fd % CHAR_BIT)) & 1) close (duplicated_fd); errno = saved_errno; } # if REPLACE_FCHDIR if (0 <= result) result = _gl_register_dup (oldfd, result); # endif return result; } #endif /* W32 */ #ifdef __KLIBC__ # define INCL_DOS # include static int klibc_fcntl (int fd, int action, /* arg */...) { va_list arg_ptr; int arg; struct stat sbuf; int result = -1; va_start (arg_ptr, action); arg = va_arg (arg_ptr, int); result = fcntl (fd, action, arg); /* EPERM for F_DUPFD, ENOTSUP for others */ if (result == -1 && (errno == EPERM || errno == ENOTSUP) && !fstat (fd, &sbuf) && S_ISDIR (sbuf.st_mode)) { ULONG ulMode; switch (action) { case F_DUPFD: /* Find available fd */ while (fcntl (arg, F_GETFL) != -1 || errno != EBADF) arg++; result = dup2 (fd, arg); break; /* Using underlying APIs is right ? */ case F_GETFD: if (DosQueryFHState (fd, &ulMode)) break; result = (ulMode & OPEN_FLAGS_NOINHERIT) ? FD_CLOEXEC : 0; break; case F_SETFD: if (arg & ~FD_CLOEXEC) break; if (DosQueryFHState (fd, &ulMode)) break; if (arg & FD_CLOEXEC) ulMode |= OPEN_FLAGS_NOINHERIT; else ulMode &= ~OPEN_FLAGS_NOINHERIT; /* Filter supported flags. */ ulMode &= (OPEN_FLAGS_WRITE_THROUGH | OPEN_FLAGS_FAIL_ON_ERROR | OPEN_FLAGS_NO_CACHE | OPEN_FLAGS_NOINHERIT); if (DosSetFHState (fd, ulMode)) break; result = 0; break; case F_GETFL: result = 0; break; case F_SETFL: if (arg != 0) break; result = 0; break; default : errno = EINVAL; break; } } va_end (arg_ptr); return result; } # define fcntl klibc_fcntl #endif /* Perform the specified ACTION on the file descriptor FD, possibly using the argument ARG further described below. This replacement handles the following actions, and forwards all others on to the native fcntl. An unrecognized ACTION returns -1 with errno set to EINVAL. F_DUPFD - duplicate FD, with int ARG being the minimum target fd. If successful, return the duplicate, which will be inheritable; otherwise return -1 and set errno. F_DUPFD_CLOEXEC - duplicate FD, with int ARG being the minimum target fd. If successful, return the duplicate, which will not be inheritable; otherwise return -1 and set errno. F_GETFD - ARG need not be present. If successful, return a non-negative value containing the descriptor flags of FD (only FD_CLOEXEC is portable, but other flags may be present); otherwise return -1 and set errno. */ int rpl_fcntl (int fd, int action, /* arg */...) { va_list arg; int result = -1; va_start (arg, action); switch (action) { #if !HAVE_FCNTL case F_DUPFD: { int target = va_arg (arg, int); result = dupfd (fd, target, 0); break; } #elif FCNTL_DUPFD_BUGGY || REPLACE_FCHDIR case F_DUPFD: { int target = va_arg (arg, int); /* Detect invalid target; needed for cygwin 1.5.x. */ if (target < 0 || getdtablesize () <= target) errno = EINVAL; else { /* Haiku alpha 2 loses fd flags on original. */ int flags = fcntl (fd, F_GETFD); if (flags < 0) { result = -1; break; } result = fcntl (fd, action, target); if (0 <= result && fcntl (fd, F_SETFD, flags) == -1) { int saved_errno = errno; close (result); result = -1; errno = saved_errno; } # if REPLACE_FCHDIR if (0 <= result) result = _gl_register_dup (fd, result); # endif } break; } /* F_DUPFD */ #endif /* FCNTL_DUPFD_BUGGY || REPLACE_FCHDIR */ case F_DUPFD_CLOEXEC: { int target = va_arg (arg, int); #if !HAVE_FCNTL result = dupfd (fd, target, O_CLOEXEC); break; #else /* HAVE_FCNTL */ /* Try the system call first, if the headers claim it exists (that is, if GNULIB_defined_F_DUPFD_CLOEXEC is 0), since we may be running with a glibc that has the macro but with an older kernel that does not support it. Cache the information on whether the system call really works, but avoid caching failure if the corresponding F_DUPFD fails for any reason. 0 = unknown, 1 = yes, -1 = no. */ static int have_dupfd_cloexec = GNULIB_defined_F_DUPFD_CLOEXEC ? -1 : 0; if (0 <= have_dupfd_cloexec) { result = fcntl (fd, action, target); if (0 <= result || errno != EINVAL) { have_dupfd_cloexec = 1; # if REPLACE_FCHDIR if (0 <= result) result = _gl_register_dup (fd, result); # endif } else { result = rpl_fcntl (fd, F_DUPFD, target); if (result < 0) break; have_dupfd_cloexec = -1; } } else result = rpl_fcntl (fd, F_DUPFD, target); if (0 <= result && have_dupfd_cloexec == -1) { int flags = fcntl (result, F_GETFD); if (flags < 0 || fcntl (result, F_SETFD, flags | FD_CLOEXEC) == -1) { int saved_errno = errno; close (result); errno = saved_errno; result = -1; } } break; #endif /* HAVE_FCNTL */ } /* F_DUPFD_CLOEXEC */ #if !HAVE_FCNTL case F_GETFD: { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ HANDLE handle = (HANDLE) _get_osfhandle (fd); DWORD flags; if (handle == INVALID_HANDLE_VALUE || GetHandleInformation (handle, &flags) == 0) errno = EBADF; else result = (flags & HANDLE_FLAG_INHERIT) ? 0 : FD_CLOEXEC; # else /* !W32 */ /* Use dup2 to reject invalid file descriptors. No way to access this information, so punt. */ if (0 <= dup2 (fd, fd)) result = 0; # endif /* !W32 */ break; } /* F_GETFD */ #endif /* !HAVE_FCNTL */ /* Implementing F_SETFD on mingw is not trivial - there is no API for changing the O_NOINHERIT bit on an fd, and merely changing the HANDLE_FLAG_INHERIT bit on the underlying handle can lead to odd state. It may be possible by duplicating the handle, using _open_osfhandle with the right flags, then using dup2 to move the duplicate onto the original, but that is not supported for now. */ default: { #if HAVE_FCNTL void *p = va_arg (arg, void *); result = fcntl (fd, action, p); #else errno = EINVAL; #endif break; } } va_end (arg); return result; } gnuastro-0.5/bootstrapped/tests/dup2.c0000644000175000017500000001161313217200022015016 00000000000000/* Duplicate an open file descriptor to a specified file descriptor. Copyright (C) 1999, 2004-2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* written by Paul Eggert */ #include /* Specification. */ #include #include #include #if HAVE_DUP2 # undef dup2 # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include # if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" # endif /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif # if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int dup2_nothrow (int fd, int desired_fd) { int result; TRY_MSVC_INVAL { result = dup2 (fd, desired_fd); } CATCH_MSVC_INVAL { errno = EBADF; result = -1; } DONE_MSVC_INVAL; return result; } # else # define dup2_nothrow dup2 # endif static int ms_windows_dup2 (int fd, int desired_fd) { int result; /* If fd is closed, mingw hangs on dup2 (fd, fd). If fd is open, dup2 (fd, fd) returns 0, but all further attempts to use fd in future dup2 calls will hang. */ if (fd == desired_fd) { if ((HANDLE) _get_osfhandle (fd) == INVALID_HANDLE_VALUE) { errno = EBADF; return -1; } return fd; } /* Wine 1.0.1 return 0 when desired_fd is negative but not -1: https://bugs.winehq.org/show_bug.cgi?id=21289 */ if (desired_fd < 0) { errno = EBADF; return -1; } result = dup2_nothrow (fd, desired_fd); if (result == 0) result = desired_fd; return result; } # define dup2 ms_windows_dup2 # elif defined __KLIBC__ # include static int klibc_dup2dirfd (int fd, int desired_fd) { int tempfd; int dupfd; tempfd = open ("NUL", O_RDONLY); if (tempfd == -1) return -1; if (tempfd == desired_fd) { close (tempfd); char path[_MAX_PATH]; if (__libc_Back_ioFHToPath (fd, path, sizeof (path))) return -1; return open(path, O_RDONLY); } dupfd = klibc_dup2dirfd (fd, desired_fd); close (tempfd); return dupfd; } static int klibc_dup2 (int fd, int desired_fd) { int dupfd; struct stat sbuf; dupfd = dup2 (fd, desired_fd); if (dupfd == -1 && errno == ENOTSUP \ && !fstat (fd, &sbuf) && S_ISDIR (sbuf.st_mode)) { close (desired_fd); return klibc_dup2dirfd (fd, desired_fd); } return dupfd; } # define dup2 klibc_dup2 # endif int rpl_dup2 (int fd, int desired_fd) { int result; # ifdef F_GETFL /* On Linux kernels 2.6.26-2.6.29, dup2 (fd, fd) returns -EBADF. On Cygwin 1.5.x, dup2 (1, 1) returns 0. On Cygwin 1.7.17, dup2 (1, -1) dumps core. On Cygwin 1.7.25, dup2 (1, 256) can dump core. On Haiku, dup2 (fd, fd) mistakenly clears FD_CLOEXEC. */ # if HAVE_SETDTABLESIZE setdtablesize (desired_fd + 1); # endif if (desired_fd < 0) fd = desired_fd; if (fd == desired_fd) return fcntl (fd, F_GETFL) == -1 ? -1 : fd; # endif result = dup2 (fd, desired_fd); /* Correct an errno value on FreeBSD 6.1 and Cygwin 1.5.x. */ if (result == -1 && errno == EMFILE) errno = EBADF; # if REPLACE_FCHDIR if (fd != desired_fd && result != -1) result = _gl_register_dup (fd, result); # endif return result; } #else /* !HAVE_DUP2 */ /* On older platforms, dup2 did not exist. */ # ifndef F_DUPFD static int dupfd (int fd, int desired_fd) { int duplicated_fd = dup (fd); if (duplicated_fd < 0 || duplicated_fd == desired_fd) return duplicated_fd; else { int r = dupfd (fd, desired_fd); int e = errno; close (duplicated_fd); errno = e; return r; } } # endif int dup2 (int fd, int desired_fd) { int result = fcntl (fd, F_GETFL) < 0 ? -1 : fd; if (result == -1 || fd == desired_fd) return result; close (desired_fd); # ifdef F_DUPFD result = fcntl (fd, F_DUPFD, desired_fd); # if REPLACE_FCHDIR if (0 <= result) result = _gl_register_dup (fd, result); # endif # else result = dupfd (fd, desired_fd); # endif if (result == -1 && (errno == EMFILE || errno == EINVAL)) errno = EBADF; return result; } #endif /* !HAVE_DUP2 */ gnuastro-0.5/bootstrapped/tests/connect.c0000644000175000017500000000301613217200022015573 00000000000000/* connect.c --- wrappers for Windows connect function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #define WIN32_LEAN_AND_MEAN /* Get winsock2.h. */ #include /* Get set_winsock_errno, FD_TO_SOCKET etc. */ #include "w32sock.h" #undef connect int rpl_connect (int fd, const struct sockaddr *sockaddr, socklen_t len) { SOCKET sock = FD_TO_SOCKET (fd); if (sock == INVALID_SOCKET) { errno = EBADF; return -1; } else { int r = connect (sock, sockaddr, len); if (r < 0) { /* EINPROGRESS is not returned by WinSock 2.0; for backwards compatibility, connect(2) uses EWOULDBLOCK. */ if (WSAGetLastError () == WSAEWOULDBLOCK) WSASetLastError (WSAEINPROGRESS); set_winsock_errno (); } return r; } } gnuastro-0.5/bootstrapped/tests/close.c0000644000175000017500000000277013217200022015255 00000000000000/* close replacement. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "fd-hook.h" #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #undef close #if HAVE_MSVC_INVALID_PARAMETER_HANDLER static int close_nothrow (int fd) { int result; TRY_MSVC_INVAL { result = close (fd); } CATCH_MSVC_INVAL { result = -1; errno = EBADF; } DONE_MSVC_INVAL; return result; } #else # define close_nothrow close #endif /* Override close() to call into other gnulib modules. */ int rpl_close (int fd) { #if WINDOWS_SOCKETS int retval = execute_all_close_hooks (close_nothrow, fd); #else int retval = close_nothrow (fd); #endif #if REPLACE_FCHDIR if (retval >= 0) _gl_unregister_fd (fd); #endif return retval; } gnuastro-0.5/bootstrapped/tests/bind.c0000644000175000017500000000240213217200022015054 00000000000000/* bind.c --- wrappers for Windows bind function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #define WIN32_LEAN_AND_MEAN /* Get winsock2.h. */ #include /* Get set_winsock_errno, FD_TO_SOCKET etc. */ #include "w32sock.h" #undef bind int rpl_bind (int fd, const struct sockaddr *sockaddr, socklen_t len) { SOCKET sock = FD_TO_SOCKET (fd); if (sock == INVALID_SOCKET) { errno = EBADF; return -1; } else { int r = bind (sock, sockaddr, len); if (r < 0) set_winsock_errno (); return r; } } gnuastro-0.5/bootstrapped/tests/accept.c0000644000175000017500000000254113217200022015403 00000000000000/* accept.c --- wrappers for Windows accept function Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paolo Bonzini */ #include #define WIN32_LEAN_AND_MEAN /* Get winsock2.h. */ #include /* Get set_winsock_errno, FD_TO_SOCKET etc. */ #include "w32sock.h" #undef accept int rpl_accept (int fd, struct sockaddr *addr, socklen_t *addrlen) { SOCKET sock = FD_TO_SOCKET (fd); if (sock == INVALID_SOCKET) { errno = EBADF; return -1; } else { SOCKET fh = accept (sock, addr, addrlen); if (fh == INVALID_SOCKET) { set_winsock_errno (); return -1; } else return SOCKET_TO_FD (fh); } } gnuastro-0.5/bootstrapped/tests/sys_socket.c0000644000175000017500000000015713217200023016334 00000000000000#include #define _GL_SYS_SOCKET_INLINE _GL_EXTERN_INLINE #include "sys/socket.h" typedef int dummy; gnuastro-0.5/bootstrapped/tests/stat-time.c0000644000175000017500000000013213217200023016046 00000000000000#include #define _GL_STAT_TIME_INLINE _GL_EXTERN_INLINE #include "stat-time.h" gnuastro-0.5/bootstrapped/tests/sockets.c0000644000175000017500000001017113217200023015616 00000000000000/* sockets.c --- wrappers for Windows socket functions Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson */ #include /* Specification. */ #include "sockets.h" #if WINDOWS_SOCKETS /* This includes winsock2.h on MinGW. */ # include # include "fd-hook.h" # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif /* Get set_winsock_errno, FD_TO_SOCKET etc. */ # include "w32sock.h" static int close_fd_maybe_socket (const struct fd_hook *remaining_list, gl_close_fn primary, int fd) { /* Note about multithread-safety: There is a race condition where, between our calls to closesocket() and the primary close(), some other thread could make system calls that allocate precisely the same HANDLE value as sock; then the primary close() would call CloseHandle() on it. */ SOCKET sock; WSANETWORKEVENTS ev; /* Test whether fd refers to a socket. */ sock = FD_TO_SOCKET (fd); ev.lNetworkEvents = 0xDEADBEEF; WSAEnumNetworkEvents (sock, NULL, &ev); if (ev.lNetworkEvents != 0xDEADBEEF) { /* fd refers to a socket. */ /* FIXME: other applications, like squid, use an undocumented _free_osfhnd free function. But this is not enough: The 'osfile' flags for fd also needs to be cleared, but it is hard to access it. Instead, here we just close twice the file descriptor. */ if (closesocket (sock)) { set_winsock_errno (); return -1; } else { /* This call frees the file descriptor and does a CloseHandle ((HANDLE) _get_osfhandle (fd)), which fails. */ _close (fd); return 0; } } else /* Some other type of file descriptor. */ return execute_close_hooks (remaining_list, primary, fd); } static int ioctl_fd_maybe_socket (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg) { SOCKET sock; WSANETWORKEVENTS ev; /* Test whether fd refers to a socket. */ sock = FD_TO_SOCKET (fd); ev.lNetworkEvents = 0xDEADBEEF; WSAEnumNetworkEvents (sock, NULL, &ev); if (ev.lNetworkEvents != 0xDEADBEEF) { /* fd refers to a socket. */ if (ioctlsocket (sock, request, arg) < 0) { set_winsock_errno (); return -1; } else return 0; } else /* Some other type of file descriptor. */ return execute_ioctl_hooks (remaining_list, primary, fd, request, arg); } static struct fd_hook fd_sockets_hook; static int initialized_sockets_version /* = 0 */; #endif /* WINDOWS_SOCKETS */ int gl_sockets_startup (int version _GL_UNUSED) { #if WINDOWS_SOCKETS if (version > initialized_sockets_version) { WSADATA data; int err; err = WSAStartup (version, &data); if (err != 0) return 1; if (data.wVersion != version) { WSACleanup (); return 2; } if (initialized_sockets_version == 0) register_fd_hook (close_fd_maybe_socket, ioctl_fd_maybe_socket, &fd_sockets_hook); initialized_sockets_version = version; } #endif return 0; } int gl_sockets_cleanup (void) { #if WINDOWS_SOCKETS int err; initialized_sockets_version = 0; unregister_fd_hook (&fd_sockets_hook); err = WSACleanup (); if (err != 0) return 1; #endif return 0; } gnuastro-0.5/bootstrapped/tests/sockets.h0000644000175000017500000000315313217200023015625 00000000000000/* sockets.h - wrappers for Windows socket functions Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson */ #ifndef SOCKETS_H #define SOCKETS_H 1 #define SOCKETS_1_0 0x0001 #define SOCKETS_1_1 0x0101 #define SOCKETS_2_0 0x0002 #define SOCKETS_2_1 0x0102 #define SOCKETS_2_2 0x0202 int gl_sockets_startup (int version) #ifndef WINDOWS_SOCKETS _GL_ATTRIBUTE_CONST #endif ; int gl_sockets_cleanup (void) #ifndef WINDOWS_SOCKETS _GL_ATTRIBUTE_CONST #endif ; /* This function is useful it you create a socket using gnulib's Winsock wrappers but needs to pass on the socket handle to some other library that only accepts sockets. */ #ifdef WINDOWS_SOCKETS # include # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif static inline SOCKET gl_fd_to_handle (int fd) { return _get_osfhandle (fd); } #else # define gl_fd_to_handle(x) (x) #endif /* WINDOWS_SOCKETS */ #endif /* SOCKETS_H */ gnuastro-0.5/bootstrapped/tests/sig-handler.c0000644000175000017500000000013213217200023016334 00000000000000#include #define SIG_HANDLER_INLINE _GL_EXTERN_INLINE #include "sig-handler.h" gnuastro-0.5/bootstrapped/tests/malloca.c0000644000175000017500000001223213217200023015553 00000000000000/* Safe automatic memory allocation. Copyright (C) 2003, 2006-2007, 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2003. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #define _GL_USE_STDLIB_ALLOC 1 #include /* Specification. */ #include "malloca.h" #include #include "verify.h" /* Silence a warning from clang's MemorySanitizer. */ #if defined __has_feature # if __has_feature(memory_sanitizer) # define NO_SANITIZE_MEMORY __attribute__((no_sanitize("memory"))) # endif #endif #ifndef NO_SANITIZE_MEMORY # define NO_SANITIZE_MEMORY #endif /* The speed critical point in this file is freea() applied to an alloca() result: it must be fast, to match the speed of alloca(). The speed of mmalloca() and freea() in the other case are not critical, because they are only invoked for big memory sizes. */ #if HAVE_ALLOCA /* Store the mmalloca() results in a hash table. This is needed to reliably distinguish a mmalloca() result and an alloca() result. Although it is possible that the same pointer is returned by alloca() and by mmalloca() at different times in the same application, it does not lead to a bug in freea(), because: - Before a pointer returned by alloca() can point into malloc()ed memory, the function must return, and once this has happened the programmer must not call freea() on it anyway. - Before a pointer returned by mmalloca() can point into the stack, it must be freed. The only function that can free it is freea(), and when freea() frees it, it also removes it from the hash table. */ #define MAGIC_NUMBER 0x1415fb4a #define MAGIC_SIZE sizeof (int) /* This is how the header info would look like without any alignment considerations. */ struct preliminary_header { void *next; int magic; }; /* But the header's size must be a multiple of sa_alignment_max. */ #define HEADER_SIZE \ (((sizeof (struct preliminary_header) + sa_alignment_max - 1) / sa_alignment_max) * sa_alignment_max) union header { void *next; struct { char room[HEADER_SIZE - MAGIC_SIZE]; int word; } magic; }; verify (HEADER_SIZE == sizeof (union header)); /* We make the hash table quite big, so that during lookups the probability of empty hash buckets is quite high. There is no need to make the hash table resizable, because when the hash table gets filled so much that the lookup becomes slow, it means that the application has memory leaks. */ #define HASH_TABLE_SIZE 257 static void * mmalloca_results[HASH_TABLE_SIZE]; #endif void * mmalloca (size_t n) { #if HAVE_ALLOCA /* Allocate one more word, that serves as an indicator for malloc()ed memory, so that freea() of an alloca() result is fast. */ size_t nplus = n + HEADER_SIZE; if (nplus >= n) { void *p = malloc (nplus); if (p != NULL) { size_t slot; union header *h = p; p = h + 1; /* Put a magic number into the indicator word. */ h->magic.word = MAGIC_NUMBER; /* Enter p into the hash table. */ slot = (uintptr_t) p % HASH_TABLE_SIZE; h->next = mmalloca_results[slot]; mmalloca_results[slot] = p; return p; } } /* Out of memory. */ return NULL; #else # if !MALLOC_0_IS_NONNULL if (n == 0) n = 1; # endif return malloc (n); #endif } #if HAVE_ALLOCA void NO_SANITIZE_MEMORY freea (void *p) { /* mmalloca() may have returned NULL. */ if (p != NULL) { /* Attempt to quickly distinguish the mmalloca() result - which has a magic indicator word - and the alloca() result - which has an uninitialized indicator word. It is for this test that sa_increment additional bytes are allocated in the alloca() case. */ if (((int *) p)[-1] == MAGIC_NUMBER) { /* Looks like a mmalloca() result. To see whether it really is one, perform a lookup in the hash table. */ size_t slot = (uintptr_t) p % HASH_TABLE_SIZE; void **chain = &mmalloca_results[slot]; for (; *chain != NULL;) { union header *h = p; if (*chain == p) { /* Found it. Remove it from the hash table and free it. */ union header *p_begin = h - 1; *chain = p_begin->next; free (p_begin); return; } h = *chain; chain = &h[-1].next; } } /* At this point, we know it was not a mmalloca() result. */ } } #endif gnuastro-0.5/bootstrapped/tests/localename.c0000644000175000017500000025136213217200023016254 00000000000000/* Determine name of the currently selected locale. Copyright (C) 1995-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Ulrich Drepper , 1995. */ /* Native Windows code written by Tor Lillqvist . */ /* Mac OS X code written by Bruno Haible . */ #include /* Specification. */ #ifdef IN_LIBINTL # include "gettextP.h" #else # include "localename.h" #endif #include #include #include #include #include #include "flexmember.h" #if HAVE_USELOCALE /* Mac OS X 10.5 defines the locale_t type in . */ # if defined __APPLE__ && defined __MACH__ # include # endif # if (__GLIBC__ >= 2 && !defined __UCLIBC__) || defined __CYGWIN__ # include # endif # if !defined IN_LIBINTL # include "glthread/lock.h" # endif # if defined __sun && HAVE_GETLOCALENAME_L /* Solaris >= 12. */ extern char * getlocalename_l(int, locale_t); # endif #endif #if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE # include # if HAVE_CFLOCALECOPYCURRENT # include # elif HAVE_CFPREFERENCESCOPYAPPVALUE # include # endif #endif #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ # define WINDOWS_NATIVE # if !defined IN_LIBINTL # include "glthread/lock.h" # endif #endif #if defined WINDOWS_NATIVE || defined __CYGWIN__ /* Native Windows or Cygwin */ # define WIN32_LEAN_AND_MEAN # include # include /* List of language codes, sorted by value: 0x01 LANG_ARABIC 0x02 LANG_BULGARIAN 0x03 LANG_CATALAN 0x04 LANG_CHINESE 0x05 LANG_CZECH 0x06 LANG_DANISH 0x07 LANG_GERMAN 0x08 LANG_GREEK 0x09 LANG_ENGLISH 0x0a LANG_SPANISH 0x0b LANG_FINNISH 0x0c LANG_FRENCH 0x0d LANG_HEBREW 0x0e LANG_HUNGARIAN 0x0f LANG_ICELANDIC 0x10 LANG_ITALIAN 0x11 LANG_JAPANESE 0x12 LANG_KOREAN 0x13 LANG_DUTCH 0x14 LANG_NORWEGIAN 0x15 LANG_POLISH 0x16 LANG_PORTUGUESE 0x17 LANG_ROMANSH 0x18 LANG_ROMANIAN 0x19 LANG_RUSSIAN 0x1a LANG_CROATIAN == LANG_SERBIAN 0x1b LANG_SLOVAK 0x1c LANG_ALBANIAN 0x1d LANG_SWEDISH 0x1e LANG_THAI 0x1f LANG_TURKISH 0x20 LANG_URDU 0x21 LANG_INDONESIAN 0x22 LANG_UKRAINIAN 0x23 LANG_BELARUSIAN 0x24 LANG_SLOVENIAN 0x25 LANG_ESTONIAN 0x26 LANG_LATVIAN 0x27 LANG_LITHUANIAN 0x28 LANG_TAJIK 0x29 LANG_FARSI 0x2a LANG_VIETNAMESE 0x2b LANG_ARMENIAN 0x2c LANG_AZERI 0x2d LANG_BASQUE 0x2e LANG_SORBIAN 0x2f LANG_MACEDONIAN 0x30 LANG_SUTU 0x31 LANG_TSONGA 0x32 LANG_TSWANA 0x33 LANG_VENDA 0x34 LANG_XHOSA 0x35 LANG_ZULU 0x36 LANG_AFRIKAANS 0x37 LANG_GEORGIAN 0x38 LANG_FAEROESE 0x39 LANG_HINDI 0x3a LANG_MALTESE 0x3b LANG_SAMI 0x3c LANG_GAELIC 0x3d LANG_YIDDISH 0x3e LANG_MALAY 0x3f LANG_KAZAK 0x40 LANG_KYRGYZ 0x41 LANG_SWAHILI 0x42 LANG_TURKMEN 0x43 LANG_UZBEK 0x44 LANG_TATAR 0x45 LANG_BENGALI 0x46 LANG_PUNJABI 0x47 LANG_GUJARATI 0x48 LANG_ORIYA 0x49 LANG_TAMIL 0x4a LANG_TELUGU 0x4b LANG_KANNADA 0x4c LANG_MALAYALAM 0x4d LANG_ASSAMESE 0x4e LANG_MARATHI 0x4f LANG_SANSKRIT 0x50 LANG_MONGOLIAN 0x51 LANG_TIBETAN 0x52 LANG_WELSH 0x53 LANG_CAMBODIAN 0x54 LANG_LAO 0x55 LANG_BURMESE 0x56 LANG_GALICIAN 0x57 LANG_KONKANI 0x58 LANG_MANIPURI 0x59 LANG_SINDHI 0x5a LANG_SYRIAC 0x5b LANG_SINHALESE 0x5c LANG_CHEROKEE 0x5d LANG_INUKTITUT 0x5e LANG_AMHARIC 0x5f LANG_TAMAZIGHT 0x60 LANG_KASHMIRI 0x61 LANG_NEPALI 0x62 LANG_FRISIAN 0x63 LANG_PASHTO 0x64 LANG_TAGALOG 0x65 LANG_DIVEHI 0x66 LANG_EDO 0x67 LANG_FULFULDE 0x68 LANG_HAUSA 0x69 LANG_IBIBIO 0x6a LANG_YORUBA 0x6d LANG_BASHKIR 0x6e LANG_LUXEMBOURGISH 0x6f LANG_GREENLANDIC 0x70 LANG_IGBO 0x71 LANG_KANURI 0x72 LANG_OROMO 0x73 LANG_TIGRINYA 0x74 LANG_GUARANI 0x75 LANG_HAWAIIAN 0x76 LANG_LATIN 0x77 LANG_SOMALI 0x78 LANG_YI 0x79 LANG_PAPIAMENTU 0x7a LANG_MAPUDUNGUN 0x7c LANG_MOHAWK 0x7e LANG_BRETON 0x82 LANG_OCCITAN 0x83 LANG_CORSICAN 0x84 LANG_ALSATIAN 0x85 LANG_YAKUT 0x86 LANG_KICHE 0x87 LANG_KINYARWANDA 0x88 LANG_WOLOF 0x8c LANG_DARI 0x91 LANG_SCOTTISH_GAELIC */ /* Mingw headers don't have latest language and sublanguage codes. */ # ifndef LANG_AFRIKAANS # define LANG_AFRIKAANS 0x36 # endif # ifndef LANG_ALBANIAN # define LANG_ALBANIAN 0x1c # endif # ifndef LANG_ALSATIAN # define LANG_ALSATIAN 0x84 # endif # ifndef LANG_AMHARIC # define LANG_AMHARIC 0x5e # endif # ifndef LANG_ARABIC # define LANG_ARABIC 0x01 # endif # ifndef LANG_ARMENIAN # define LANG_ARMENIAN 0x2b # endif # ifndef LANG_ASSAMESE # define LANG_ASSAMESE 0x4d # endif # ifndef LANG_AZERI # define LANG_AZERI 0x2c # endif # ifndef LANG_BASHKIR # define LANG_BASHKIR 0x6d # endif # ifndef LANG_BASQUE # define LANG_BASQUE 0x2d # endif # ifndef LANG_BELARUSIAN # define LANG_BELARUSIAN 0x23 # endif # ifndef LANG_BENGALI # define LANG_BENGALI 0x45 # endif # ifndef LANG_BRETON # define LANG_BRETON 0x7e # endif # ifndef LANG_BURMESE # define LANG_BURMESE 0x55 # endif # ifndef LANG_CAMBODIAN # define LANG_CAMBODIAN 0x53 # endif # ifndef LANG_CATALAN # define LANG_CATALAN 0x03 # endif # ifndef LANG_CHEROKEE # define LANG_CHEROKEE 0x5c # endif # ifndef LANG_CORSICAN # define LANG_CORSICAN 0x83 # endif # ifndef LANG_DARI # define LANG_DARI 0x8c # endif # ifndef LANG_DIVEHI # define LANG_DIVEHI 0x65 # endif # ifndef LANG_EDO # define LANG_EDO 0x66 # endif # ifndef LANG_ESTONIAN # define LANG_ESTONIAN 0x25 # endif # ifndef LANG_FAEROESE # define LANG_FAEROESE 0x38 # endif # ifndef LANG_FARSI # define LANG_FARSI 0x29 # endif # ifndef LANG_FRISIAN # define LANG_FRISIAN 0x62 # endif # ifndef LANG_FULFULDE # define LANG_FULFULDE 0x67 # endif # ifndef LANG_GAELIC # define LANG_GAELIC 0x3c # endif # ifndef LANG_GALICIAN # define LANG_GALICIAN 0x56 # endif # ifndef LANG_GEORGIAN # define LANG_GEORGIAN 0x37 # endif # ifndef LANG_GREENLANDIC # define LANG_GREENLANDIC 0x6f # endif # ifndef LANG_GUARANI # define LANG_GUARANI 0x74 # endif # ifndef LANG_GUJARATI # define LANG_GUJARATI 0x47 # endif # ifndef LANG_HAUSA # define LANG_HAUSA 0x68 # endif # ifndef LANG_HAWAIIAN # define LANG_HAWAIIAN 0x75 # endif # ifndef LANG_HEBREW # define LANG_HEBREW 0x0d # endif # ifndef LANG_HINDI # define LANG_HINDI 0x39 # endif # ifndef LANG_IBIBIO # define LANG_IBIBIO 0x69 # endif # ifndef LANG_IGBO # define LANG_IGBO 0x70 # endif # ifndef LANG_INDONESIAN # define LANG_INDONESIAN 0x21 # endif # ifndef LANG_INUKTITUT # define LANG_INUKTITUT 0x5d # endif # ifndef LANG_KANNADA # define LANG_KANNADA 0x4b # endif # ifndef LANG_KANURI # define LANG_KANURI 0x71 # endif # ifndef LANG_KASHMIRI # define LANG_KASHMIRI 0x60 # endif # ifndef LANG_KAZAK # define LANG_KAZAK 0x3f # endif # ifndef LANG_KICHE # define LANG_KICHE 0x86 # endif # ifndef LANG_KINYARWANDA # define LANG_KINYARWANDA 0x87 # endif # ifndef LANG_KONKANI # define LANG_KONKANI 0x57 # endif # ifndef LANG_KYRGYZ # define LANG_KYRGYZ 0x40 # endif # ifndef LANG_LAO # define LANG_LAO 0x54 # endif # ifndef LANG_LATIN # define LANG_LATIN 0x76 # endif # ifndef LANG_LATVIAN # define LANG_LATVIAN 0x26 # endif # ifndef LANG_LITHUANIAN # define LANG_LITHUANIAN 0x27 # endif # ifndef LANG_LUXEMBOURGISH # define LANG_LUXEMBOURGISH 0x6e # endif # ifndef LANG_MACEDONIAN # define LANG_MACEDONIAN 0x2f # endif # ifndef LANG_MALAY # define LANG_MALAY 0x3e # endif # ifndef LANG_MALAYALAM # define LANG_MALAYALAM 0x4c # endif # ifndef LANG_MALTESE # define LANG_MALTESE 0x3a # endif # ifndef LANG_MANIPURI # define LANG_MANIPURI 0x58 # endif # ifndef LANG_MAORI # define LANG_MAORI 0x81 # endif # ifndef LANG_MAPUDUNGUN # define LANG_MAPUDUNGUN 0x7a # endif # ifndef LANG_MARATHI # define LANG_MARATHI 0x4e # endif # ifndef LANG_MOHAWK # define LANG_MOHAWK 0x7c # endif # ifndef LANG_MONGOLIAN # define LANG_MONGOLIAN 0x50 # endif # ifndef LANG_NEPALI # define LANG_NEPALI 0x61 # endif # ifndef LANG_OCCITAN # define LANG_OCCITAN 0x82 # endif # ifndef LANG_ORIYA # define LANG_ORIYA 0x48 # endif # ifndef LANG_OROMO # define LANG_OROMO 0x72 # endif # ifndef LANG_PAPIAMENTU # define LANG_PAPIAMENTU 0x79 # endif # ifndef LANG_PASHTO # define LANG_PASHTO 0x63 # endif # ifndef LANG_PUNJABI # define LANG_PUNJABI 0x46 # endif # ifndef LANG_QUECHUA # define LANG_QUECHUA 0x6b # endif # ifndef LANG_ROMANSH # define LANG_ROMANSH 0x17 # endif # ifndef LANG_SAMI # define LANG_SAMI 0x3b # endif # ifndef LANG_SANSKRIT # define LANG_SANSKRIT 0x4f # endif # ifndef LANG_SCOTTISH_GAELIC # define LANG_SCOTTISH_GAELIC 0x91 # endif # ifndef LANG_SERBIAN # define LANG_SERBIAN 0x1a # endif # ifndef LANG_SINDHI # define LANG_SINDHI 0x59 # endif # ifndef LANG_SINHALESE # define LANG_SINHALESE 0x5b # endif # ifndef LANG_SLOVAK # define LANG_SLOVAK 0x1b # endif # ifndef LANG_SOMALI # define LANG_SOMALI 0x77 # endif # ifndef LANG_SORBIAN # define LANG_SORBIAN 0x2e # endif # ifndef LANG_SOTHO # define LANG_SOTHO 0x6c # endif # ifndef LANG_SUTU # define LANG_SUTU 0x30 # endif # ifndef LANG_SWAHILI # define LANG_SWAHILI 0x41 # endif # ifndef LANG_SYRIAC # define LANG_SYRIAC 0x5a # endif # ifndef LANG_TAGALOG # define LANG_TAGALOG 0x64 # endif # ifndef LANG_TAJIK # define LANG_TAJIK 0x28 # endif # ifndef LANG_TAMAZIGHT # define LANG_TAMAZIGHT 0x5f # endif # ifndef LANG_TAMIL # define LANG_TAMIL 0x49 # endif # ifndef LANG_TATAR # define LANG_TATAR 0x44 # endif # ifndef LANG_TELUGU # define LANG_TELUGU 0x4a # endif # ifndef LANG_THAI # define LANG_THAI 0x1e # endif # ifndef LANG_TIBETAN # define LANG_TIBETAN 0x51 # endif # ifndef LANG_TIGRINYA # define LANG_TIGRINYA 0x73 # endif # ifndef LANG_TSONGA # define LANG_TSONGA 0x31 # endif # ifndef LANG_TSWANA # define LANG_TSWANA 0x32 # endif # ifndef LANG_TURKMEN # define LANG_TURKMEN 0x42 # endif # ifndef LANG_UIGHUR # define LANG_UIGHUR 0x80 # endif # ifndef LANG_UKRAINIAN # define LANG_UKRAINIAN 0x22 # endif # ifndef LANG_URDU # define LANG_URDU 0x20 # endif # ifndef LANG_UZBEK # define LANG_UZBEK 0x43 # endif # ifndef LANG_VENDA # define LANG_VENDA 0x33 # endif # ifndef LANG_VIETNAMESE # define LANG_VIETNAMESE 0x2a # endif # ifndef LANG_WELSH # define LANG_WELSH 0x52 # endif # ifndef LANG_WOLOF # define LANG_WOLOF 0x88 # endif # ifndef LANG_XHOSA # define LANG_XHOSA 0x34 # endif # ifndef LANG_YAKUT # define LANG_YAKUT 0x85 # endif # ifndef LANG_YI # define LANG_YI 0x78 # endif # ifndef LANG_YIDDISH # define LANG_YIDDISH 0x3d # endif # ifndef LANG_YORUBA # define LANG_YORUBA 0x6a # endif # ifndef LANG_ZULU # define LANG_ZULU 0x35 # endif # ifndef SUBLANG_AFRIKAANS_SOUTH_AFRICA # define SUBLANG_AFRIKAANS_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_ALBANIAN_ALBANIA # define SUBLANG_ALBANIAN_ALBANIA 0x01 # endif # ifndef SUBLANG_ALSATIAN_FRANCE # define SUBLANG_ALSATIAN_FRANCE 0x01 # endif # ifndef SUBLANG_AMHARIC_ETHIOPIA # define SUBLANG_AMHARIC_ETHIOPIA 0x01 # endif # ifndef SUBLANG_ARABIC_SAUDI_ARABIA # define SUBLANG_ARABIC_SAUDI_ARABIA 0x01 # endif # ifndef SUBLANG_ARABIC_IRAQ # define SUBLANG_ARABIC_IRAQ 0x02 # endif # ifndef SUBLANG_ARABIC_EGYPT # define SUBLANG_ARABIC_EGYPT 0x03 # endif # ifndef SUBLANG_ARABIC_LIBYA # define SUBLANG_ARABIC_LIBYA 0x04 # endif # ifndef SUBLANG_ARABIC_ALGERIA # define SUBLANG_ARABIC_ALGERIA 0x05 # endif # ifndef SUBLANG_ARABIC_MOROCCO # define SUBLANG_ARABIC_MOROCCO 0x06 # endif # ifndef SUBLANG_ARABIC_TUNISIA # define SUBLANG_ARABIC_TUNISIA 0x07 # endif # ifndef SUBLANG_ARABIC_OMAN # define SUBLANG_ARABIC_OMAN 0x08 # endif # ifndef SUBLANG_ARABIC_YEMEN # define SUBLANG_ARABIC_YEMEN 0x09 # endif # ifndef SUBLANG_ARABIC_SYRIA # define SUBLANG_ARABIC_SYRIA 0x0a # endif # ifndef SUBLANG_ARABIC_JORDAN # define SUBLANG_ARABIC_JORDAN 0x0b # endif # ifndef SUBLANG_ARABIC_LEBANON # define SUBLANG_ARABIC_LEBANON 0x0c # endif # ifndef SUBLANG_ARABIC_KUWAIT # define SUBLANG_ARABIC_KUWAIT 0x0d # endif # ifndef SUBLANG_ARABIC_UAE # define SUBLANG_ARABIC_UAE 0x0e # endif # ifndef SUBLANG_ARABIC_BAHRAIN # define SUBLANG_ARABIC_BAHRAIN 0x0f # endif # ifndef SUBLANG_ARABIC_QATAR # define SUBLANG_ARABIC_QATAR 0x10 # endif # ifndef SUBLANG_ARMENIAN_ARMENIA # define SUBLANG_ARMENIAN_ARMENIA 0x01 # endif # ifndef SUBLANG_ASSAMESE_INDIA # define SUBLANG_ASSAMESE_INDIA 0x01 # endif # ifndef SUBLANG_AZERI_LATIN # define SUBLANG_AZERI_LATIN 0x01 # endif # ifndef SUBLANG_AZERI_CYRILLIC # define SUBLANG_AZERI_CYRILLIC 0x02 # endif # ifndef SUBLANG_BASHKIR_RUSSIA # define SUBLANG_BASHKIR_RUSSIA 0x01 # endif # ifndef SUBLANG_BASQUE_BASQUE # define SUBLANG_BASQUE_BASQUE 0x01 # endif # ifndef SUBLANG_BELARUSIAN_BELARUS # define SUBLANG_BELARUSIAN_BELARUS 0x01 # endif # ifndef SUBLANG_BENGALI_INDIA # define SUBLANG_BENGALI_INDIA 0x01 # endif # ifndef SUBLANG_BENGALI_BANGLADESH # define SUBLANG_BENGALI_BANGLADESH 0x02 # endif # ifndef SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_LATIN # define SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_LATIN 0x05 # endif # ifndef SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_CYRILLIC # define SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_CYRILLIC 0x08 # endif # ifndef SUBLANG_BRETON_FRANCE # define SUBLANG_BRETON_FRANCE 0x01 # endif # ifndef SUBLANG_BULGARIAN_BULGARIA # define SUBLANG_BULGARIAN_BULGARIA 0x01 # endif # ifndef SUBLANG_CAMBODIAN_CAMBODIA # define SUBLANG_CAMBODIAN_CAMBODIA 0x01 # endif # ifndef SUBLANG_CATALAN_SPAIN # define SUBLANG_CATALAN_SPAIN 0x01 # endif # ifndef SUBLANG_CORSICAN_FRANCE # define SUBLANG_CORSICAN_FRANCE 0x01 # endif # ifndef SUBLANG_CROATIAN_CROATIA # define SUBLANG_CROATIAN_CROATIA 0x01 # endif # ifndef SUBLANG_CROATIAN_BOSNIA_HERZEGOVINA_LATIN # define SUBLANG_CROATIAN_BOSNIA_HERZEGOVINA_LATIN 0x04 # endif # ifndef SUBLANG_CHINESE_MACAU # define SUBLANG_CHINESE_MACAU 0x05 # endif # ifndef SUBLANG_CZECH_CZECH_REPUBLIC # define SUBLANG_CZECH_CZECH_REPUBLIC 0x01 # endif # ifndef SUBLANG_DANISH_DENMARK # define SUBLANG_DANISH_DENMARK 0x01 # endif # ifndef SUBLANG_DARI_AFGHANISTAN # define SUBLANG_DARI_AFGHANISTAN 0x01 # endif # ifndef SUBLANG_DIVEHI_MALDIVES # define SUBLANG_DIVEHI_MALDIVES 0x01 # endif # ifndef SUBLANG_DUTCH_SURINAM # define SUBLANG_DUTCH_SURINAM 0x03 # endif # ifndef SUBLANG_ENGLISH_SOUTH_AFRICA # define SUBLANG_ENGLISH_SOUTH_AFRICA 0x07 # endif # ifndef SUBLANG_ENGLISH_JAMAICA # define SUBLANG_ENGLISH_JAMAICA 0x08 # endif # ifndef SUBLANG_ENGLISH_CARIBBEAN # define SUBLANG_ENGLISH_CARIBBEAN 0x09 # endif # ifndef SUBLANG_ENGLISH_BELIZE # define SUBLANG_ENGLISH_BELIZE 0x0a # endif # ifndef SUBLANG_ENGLISH_TRINIDAD # define SUBLANG_ENGLISH_TRINIDAD 0x0b # endif # ifndef SUBLANG_ENGLISH_ZIMBABWE # define SUBLANG_ENGLISH_ZIMBABWE 0x0c # endif # ifndef SUBLANG_ENGLISH_PHILIPPINES # define SUBLANG_ENGLISH_PHILIPPINES 0x0d # endif # ifndef SUBLANG_ENGLISH_INDONESIA # define SUBLANG_ENGLISH_INDONESIA 0x0e # endif # ifndef SUBLANG_ENGLISH_HONGKONG # define SUBLANG_ENGLISH_HONGKONG 0x0f # endif # ifndef SUBLANG_ENGLISH_INDIA # define SUBLANG_ENGLISH_INDIA 0x10 # endif # ifndef SUBLANG_ENGLISH_MALAYSIA # define SUBLANG_ENGLISH_MALAYSIA 0x11 # endif # ifndef SUBLANG_ENGLISH_SINGAPORE # define SUBLANG_ENGLISH_SINGAPORE 0x12 # endif # ifndef SUBLANG_ESTONIAN_ESTONIA # define SUBLANG_ESTONIAN_ESTONIA 0x01 # endif # ifndef SUBLANG_FAEROESE_FAROE_ISLANDS # define SUBLANG_FAEROESE_FAROE_ISLANDS 0x01 # endif # ifndef SUBLANG_FARSI_IRAN # define SUBLANG_FARSI_IRAN 0x01 # endif # ifndef SUBLANG_FINNISH_FINLAND # define SUBLANG_FINNISH_FINLAND 0x01 # endif # ifndef SUBLANG_FRENCH_LUXEMBOURG # define SUBLANG_FRENCH_LUXEMBOURG 0x05 # endif # ifndef SUBLANG_FRENCH_MONACO # define SUBLANG_FRENCH_MONACO 0x06 # endif # ifndef SUBLANG_FRENCH_WESTINDIES # define SUBLANG_FRENCH_WESTINDIES 0x07 # endif # ifndef SUBLANG_FRENCH_REUNION # define SUBLANG_FRENCH_REUNION 0x08 # endif # ifndef SUBLANG_FRENCH_CONGO # define SUBLANG_FRENCH_CONGO 0x09 # endif # ifndef SUBLANG_FRENCH_SENEGAL # define SUBLANG_FRENCH_SENEGAL 0x0a # endif # ifndef SUBLANG_FRENCH_CAMEROON # define SUBLANG_FRENCH_CAMEROON 0x0b # endif # ifndef SUBLANG_FRENCH_COTEDIVOIRE # define SUBLANG_FRENCH_COTEDIVOIRE 0x0c # endif # ifndef SUBLANG_FRENCH_MALI # define SUBLANG_FRENCH_MALI 0x0d # endif # ifndef SUBLANG_FRENCH_MOROCCO # define SUBLANG_FRENCH_MOROCCO 0x0e # endif # ifndef SUBLANG_FRENCH_HAITI # define SUBLANG_FRENCH_HAITI 0x0f # endif # ifndef SUBLANG_FRISIAN_NETHERLANDS # define SUBLANG_FRISIAN_NETHERLANDS 0x01 # endif # ifndef SUBLANG_GALICIAN_SPAIN # define SUBLANG_GALICIAN_SPAIN 0x01 # endif # ifndef SUBLANG_GEORGIAN_GEORGIA # define SUBLANG_GEORGIAN_GEORGIA 0x01 # endif # ifndef SUBLANG_GERMAN_LUXEMBOURG # define SUBLANG_GERMAN_LUXEMBOURG 0x04 # endif # ifndef SUBLANG_GERMAN_LIECHTENSTEIN # define SUBLANG_GERMAN_LIECHTENSTEIN 0x05 # endif # ifndef SUBLANG_GREEK_GREECE # define SUBLANG_GREEK_GREECE 0x01 # endif # ifndef SUBLANG_GREENLANDIC_GREENLAND # define SUBLANG_GREENLANDIC_GREENLAND 0x01 # endif # ifndef SUBLANG_GUJARATI_INDIA # define SUBLANG_GUJARATI_INDIA 0x01 # endif # ifndef SUBLANG_HAUSA_NIGERIA_LATIN # define SUBLANG_HAUSA_NIGERIA_LATIN 0x01 # endif # ifndef SUBLANG_HEBREW_ISRAEL # define SUBLANG_HEBREW_ISRAEL 0x01 # endif # ifndef SUBLANG_HINDI_INDIA # define SUBLANG_HINDI_INDIA 0x01 # endif # ifndef SUBLANG_HUNGARIAN_HUNGARY # define SUBLANG_HUNGARIAN_HUNGARY 0x01 # endif # ifndef SUBLANG_ICELANDIC_ICELAND # define SUBLANG_ICELANDIC_ICELAND 0x01 # endif # ifndef SUBLANG_IGBO_NIGERIA # define SUBLANG_IGBO_NIGERIA 0x01 # endif # ifndef SUBLANG_INDONESIAN_INDONESIA # define SUBLANG_INDONESIAN_INDONESIA 0x01 # endif # ifndef SUBLANG_INUKTITUT_CANADA # define SUBLANG_INUKTITUT_CANADA 0x01 # endif # undef SUBLANG_INUKTITUT_CANADA_LATIN # define SUBLANG_INUKTITUT_CANADA_LATIN 0x02 # undef SUBLANG_IRISH_IRELAND # define SUBLANG_IRISH_IRELAND 0x02 # ifndef SUBLANG_JAPANESE_JAPAN # define SUBLANG_JAPANESE_JAPAN 0x01 # endif # ifndef SUBLANG_KANNADA_INDIA # define SUBLANG_KANNADA_INDIA 0x01 # endif # ifndef SUBLANG_KASHMIRI_INDIA # define SUBLANG_KASHMIRI_INDIA 0x02 # endif # ifndef SUBLANG_KAZAK_KAZAKHSTAN # define SUBLANG_KAZAK_KAZAKHSTAN 0x01 # endif # ifndef SUBLANG_KICHE_GUATEMALA # define SUBLANG_KICHE_GUATEMALA 0x01 # endif # ifndef SUBLANG_KINYARWANDA_RWANDA # define SUBLANG_KINYARWANDA_RWANDA 0x01 # endif # ifndef SUBLANG_KONKANI_INDIA # define SUBLANG_KONKANI_INDIA 0x01 # endif # ifndef SUBLANG_KYRGYZ_KYRGYZSTAN # define SUBLANG_KYRGYZ_KYRGYZSTAN 0x01 # endif # ifndef SUBLANG_LAO_LAOS # define SUBLANG_LAO_LAOS 0x01 # endif # ifndef SUBLANG_LATVIAN_LATVIA # define SUBLANG_LATVIAN_LATVIA 0x01 # endif # ifndef SUBLANG_LITHUANIAN_LITHUANIA # define SUBLANG_LITHUANIAN_LITHUANIA 0x01 # endif # undef SUBLANG_LOWER_SORBIAN_GERMANY # define SUBLANG_LOWER_SORBIAN_GERMANY 0x02 # ifndef SUBLANG_LUXEMBOURGISH_LUXEMBOURG # define SUBLANG_LUXEMBOURGISH_LUXEMBOURG 0x01 # endif # ifndef SUBLANG_MACEDONIAN_MACEDONIA # define SUBLANG_MACEDONIAN_MACEDONIA 0x01 # endif # ifndef SUBLANG_MALAY_MALAYSIA # define SUBLANG_MALAY_MALAYSIA 0x01 # endif # ifndef SUBLANG_MALAY_BRUNEI_DARUSSALAM # define SUBLANG_MALAY_BRUNEI_DARUSSALAM 0x02 # endif # ifndef SUBLANG_MALAYALAM_INDIA # define SUBLANG_MALAYALAM_INDIA 0x01 # endif # ifndef SUBLANG_MALTESE_MALTA # define SUBLANG_MALTESE_MALTA 0x01 # endif # ifndef SUBLANG_MAORI_NEW_ZEALAND # define SUBLANG_MAORI_NEW_ZEALAND 0x01 # endif # ifndef SUBLANG_MAPUDUNGUN_CHILE # define SUBLANG_MAPUDUNGUN_CHILE 0x01 # endif # ifndef SUBLANG_MARATHI_INDIA # define SUBLANG_MARATHI_INDIA 0x01 # endif # ifndef SUBLANG_MOHAWK_CANADA # define SUBLANG_MOHAWK_CANADA 0x01 # endif # ifndef SUBLANG_MONGOLIAN_CYRILLIC_MONGOLIA # define SUBLANG_MONGOLIAN_CYRILLIC_MONGOLIA 0x01 # endif # ifndef SUBLANG_MONGOLIAN_PRC # define SUBLANG_MONGOLIAN_PRC 0x02 # endif # ifndef SUBLANG_NEPALI_NEPAL # define SUBLANG_NEPALI_NEPAL 0x01 # endif # ifndef SUBLANG_NEPALI_INDIA # define SUBLANG_NEPALI_INDIA 0x02 # endif # ifndef SUBLANG_OCCITAN_FRANCE # define SUBLANG_OCCITAN_FRANCE 0x01 # endif # ifndef SUBLANG_ORIYA_INDIA # define SUBLANG_ORIYA_INDIA 0x01 # endif # ifndef SUBLANG_PASHTO_AFGHANISTAN # define SUBLANG_PASHTO_AFGHANISTAN 0x01 # endif # ifndef SUBLANG_POLISH_POLAND # define SUBLANG_POLISH_POLAND 0x01 # endif # ifndef SUBLANG_PUNJABI_INDIA # define SUBLANG_PUNJABI_INDIA 0x01 # endif # ifndef SUBLANG_PUNJABI_PAKISTAN # define SUBLANG_PUNJABI_PAKISTAN 0x02 # endif # ifndef SUBLANG_QUECHUA_BOLIVIA # define SUBLANG_QUECHUA_BOLIVIA 0x01 # endif # ifndef SUBLANG_QUECHUA_ECUADOR # define SUBLANG_QUECHUA_ECUADOR 0x02 # endif # ifndef SUBLANG_QUECHUA_PERU # define SUBLANG_QUECHUA_PERU 0x03 # endif # ifndef SUBLANG_ROMANIAN_ROMANIA # define SUBLANG_ROMANIAN_ROMANIA 0x01 # endif # ifndef SUBLANG_ROMANIAN_MOLDOVA # define SUBLANG_ROMANIAN_MOLDOVA 0x02 # endif # ifndef SUBLANG_ROMANSH_SWITZERLAND # define SUBLANG_ROMANSH_SWITZERLAND 0x01 # endif # ifndef SUBLANG_RUSSIAN_RUSSIA # define SUBLANG_RUSSIAN_RUSSIA 0x01 # endif # ifndef SUBLANG_RUSSIAN_MOLDAVIA # define SUBLANG_RUSSIAN_MOLDAVIA 0x02 # endif # ifndef SUBLANG_SAMI_NORTHERN_NORWAY # define SUBLANG_SAMI_NORTHERN_NORWAY 0x01 # endif # ifndef SUBLANG_SAMI_NORTHERN_SWEDEN # define SUBLANG_SAMI_NORTHERN_SWEDEN 0x02 # endif # ifndef SUBLANG_SAMI_NORTHERN_FINLAND # define SUBLANG_SAMI_NORTHERN_FINLAND 0x03 # endif # ifndef SUBLANG_SAMI_LULE_NORWAY # define SUBLANG_SAMI_LULE_NORWAY 0x04 # endif # ifndef SUBLANG_SAMI_LULE_SWEDEN # define SUBLANG_SAMI_LULE_SWEDEN 0x05 # endif # ifndef SUBLANG_SAMI_SOUTHERN_NORWAY # define SUBLANG_SAMI_SOUTHERN_NORWAY 0x06 # endif # ifndef SUBLANG_SAMI_SOUTHERN_SWEDEN # define SUBLANG_SAMI_SOUTHERN_SWEDEN 0x07 # endif # undef SUBLANG_SAMI_SKOLT_FINLAND # define SUBLANG_SAMI_SKOLT_FINLAND 0x08 # undef SUBLANG_SAMI_INARI_FINLAND # define SUBLANG_SAMI_INARI_FINLAND 0x09 # ifndef SUBLANG_SANSKRIT_INDIA # define SUBLANG_SANSKRIT_INDIA 0x01 # endif # ifndef SUBLANG_SERBIAN_LATIN # define SUBLANG_SERBIAN_LATIN 0x02 # endif # ifndef SUBLANG_SERBIAN_CYRILLIC # define SUBLANG_SERBIAN_CYRILLIC 0x03 # endif # ifndef SUBLANG_SINDHI_INDIA # define SUBLANG_SINDHI_INDIA 0x01 # endif # undef SUBLANG_SINDHI_PAKISTAN # define SUBLANG_SINDHI_PAKISTAN 0x02 # ifndef SUBLANG_SINDHI_AFGHANISTAN # define SUBLANG_SINDHI_AFGHANISTAN 0x02 # endif # ifndef SUBLANG_SINHALESE_SRI_LANKA # define SUBLANG_SINHALESE_SRI_LANKA 0x01 # endif # ifndef SUBLANG_SLOVAK_SLOVAKIA # define SUBLANG_SLOVAK_SLOVAKIA 0x01 # endif # ifndef SUBLANG_SLOVENIAN_SLOVENIA # define SUBLANG_SLOVENIAN_SLOVENIA 0x01 # endif # ifndef SUBLANG_SOTHO_SOUTH_AFRICA # define SUBLANG_SOTHO_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_SPANISH_GUATEMALA # define SUBLANG_SPANISH_GUATEMALA 0x04 # endif # ifndef SUBLANG_SPANISH_COSTA_RICA # define SUBLANG_SPANISH_COSTA_RICA 0x05 # endif # ifndef SUBLANG_SPANISH_PANAMA # define SUBLANG_SPANISH_PANAMA 0x06 # endif # ifndef SUBLANG_SPANISH_DOMINICAN_REPUBLIC # define SUBLANG_SPANISH_DOMINICAN_REPUBLIC 0x07 # endif # ifndef SUBLANG_SPANISH_VENEZUELA # define SUBLANG_SPANISH_VENEZUELA 0x08 # endif # ifndef SUBLANG_SPANISH_COLOMBIA # define SUBLANG_SPANISH_COLOMBIA 0x09 # endif # ifndef SUBLANG_SPANISH_PERU # define SUBLANG_SPANISH_PERU 0x0a # endif # ifndef SUBLANG_SPANISH_ARGENTINA # define SUBLANG_SPANISH_ARGENTINA 0x0b # endif # ifndef SUBLANG_SPANISH_ECUADOR # define SUBLANG_SPANISH_ECUADOR 0x0c # endif # ifndef SUBLANG_SPANISH_CHILE # define SUBLANG_SPANISH_CHILE 0x0d # endif # ifndef SUBLANG_SPANISH_URUGUAY # define SUBLANG_SPANISH_URUGUAY 0x0e # endif # ifndef SUBLANG_SPANISH_PARAGUAY # define SUBLANG_SPANISH_PARAGUAY 0x0f # endif # ifndef SUBLANG_SPANISH_BOLIVIA # define SUBLANG_SPANISH_BOLIVIA 0x10 # endif # ifndef SUBLANG_SPANISH_EL_SALVADOR # define SUBLANG_SPANISH_EL_SALVADOR 0x11 # endif # ifndef SUBLANG_SPANISH_HONDURAS # define SUBLANG_SPANISH_HONDURAS 0x12 # endif # ifndef SUBLANG_SPANISH_NICARAGUA # define SUBLANG_SPANISH_NICARAGUA 0x13 # endif # ifndef SUBLANG_SPANISH_PUERTO_RICO # define SUBLANG_SPANISH_PUERTO_RICO 0x14 # endif # ifndef SUBLANG_SPANISH_US # define SUBLANG_SPANISH_US 0x15 # endif # ifndef SUBLANG_SWAHILI_KENYA # define SUBLANG_SWAHILI_KENYA 0x01 # endif # ifndef SUBLANG_SWEDISH_SWEDEN # define SUBLANG_SWEDISH_SWEDEN 0x01 # endif # ifndef SUBLANG_SWEDISH_FINLAND # define SUBLANG_SWEDISH_FINLAND 0x02 # endif # ifndef SUBLANG_SYRIAC_SYRIA # define SUBLANG_SYRIAC_SYRIA 0x01 # endif # ifndef SUBLANG_TAGALOG_PHILIPPINES # define SUBLANG_TAGALOG_PHILIPPINES 0x01 # endif # ifndef SUBLANG_TAJIK_TAJIKISTAN # define SUBLANG_TAJIK_TAJIKISTAN 0x01 # endif # ifndef SUBLANG_TAMAZIGHT_ARABIC # define SUBLANG_TAMAZIGHT_ARABIC 0x01 # endif # ifndef SUBLANG_TAMAZIGHT_ALGERIA_LATIN # define SUBLANG_TAMAZIGHT_ALGERIA_LATIN 0x02 # endif # ifndef SUBLANG_TAMIL_INDIA # define SUBLANG_TAMIL_INDIA 0x01 # endif # ifndef SUBLANG_TATAR_RUSSIA # define SUBLANG_TATAR_RUSSIA 0x01 # endif # ifndef SUBLANG_TELUGU_INDIA # define SUBLANG_TELUGU_INDIA 0x01 # endif # ifndef SUBLANG_THAI_THAILAND # define SUBLANG_THAI_THAILAND 0x01 # endif # ifndef SUBLANG_TIBETAN_PRC # define SUBLANG_TIBETAN_PRC 0x01 # endif # undef SUBLANG_TIBETAN_BHUTAN # define SUBLANG_TIBETAN_BHUTAN 0x02 # ifndef SUBLANG_TIGRINYA_ETHIOPIA # define SUBLANG_TIGRINYA_ETHIOPIA 0x01 # endif # ifndef SUBLANG_TIGRINYA_ERITREA # define SUBLANG_TIGRINYA_ERITREA 0x02 # endif # ifndef SUBLANG_TSWANA_SOUTH_AFRICA # define SUBLANG_TSWANA_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_TURKISH_TURKEY # define SUBLANG_TURKISH_TURKEY 0x01 # endif # ifndef SUBLANG_TURKMEN_TURKMENISTAN # define SUBLANG_TURKMEN_TURKMENISTAN 0x01 # endif # ifndef SUBLANG_UIGHUR_PRC # define SUBLANG_UIGHUR_PRC 0x01 # endif # ifndef SUBLANG_UKRAINIAN_UKRAINE # define SUBLANG_UKRAINIAN_UKRAINE 0x01 # endif # ifndef SUBLANG_UPPER_SORBIAN_GERMANY # define SUBLANG_UPPER_SORBIAN_GERMANY 0x01 # endif # ifndef SUBLANG_URDU_PAKISTAN # define SUBLANG_URDU_PAKISTAN 0x01 # endif # ifndef SUBLANG_URDU_INDIA # define SUBLANG_URDU_INDIA 0x02 # endif # ifndef SUBLANG_UZBEK_LATIN # define SUBLANG_UZBEK_LATIN 0x01 # endif # ifndef SUBLANG_UZBEK_CYRILLIC # define SUBLANG_UZBEK_CYRILLIC 0x02 # endif # ifndef SUBLANG_VIETNAMESE_VIETNAM # define SUBLANG_VIETNAMESE_VIETNAM 0x01 # endif # ifndef SUBLANG_WELSH_UNITED_KINGDOM # define SUBLANG_WELSH_UNITED_KINGDOM 0x01 # endif # ifndef SUBLANG_WOLOF_SENEGAL # define SUBLANG_WOLOF_SENEGAL 0x01 # endif # ifndef SUBLANG_XHOSA_SOUTH_AFRICA # define SUBLANG_XHOSA_SOUTH_AFRICA 0x01 # endif # ifndef SUBLANG_YAKUT_RUSSIA # define SUBLANG_YAKUT_RUSSIA 0x01 # endif # ifndef SUBLANG_YI_PRC # define SUBLANG_YI_PRC 0x01 # endif # ifndef SUBLANG_YORUBA_NIGERIA # define SUBLANG_YORUBA_NIGERIA 0x01 # endif # ifndef SUBLANG_ZULU_SOUTH_AFRICA # define SUBLANG_ZULU_SOUTH_AFRICA 0x01 # endif /* GetLocaleInfoA operations. */ # ifndef LOCALE_SNAME # define LOCALE_SNAME 0x5c # endif # ifndef LOCALE_NAME_MAX_LENGTH # define LOCALE_NAME_MAX_LENGTH 85 # endif #endif #if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer */ /* Canonicalize a Mac OS X locale name to a Unix locale name. NAME is a sufficiently large buffer. On input, it contains the Mac OS X locale name. On output, it contains the Unix locale name. */ # if !defined IN_LIBINTL static # endif void gl_locale_name_canonicalize (char *name) { /* This conversion is based on a posting by Deborah GoldSmith on 2005-03-08, https://lists.apple.com/archives/carbon-dev/2005/Mar/msg00293.html */ /* Convert legacy (NeXTstep inherited) English names to Unix (ISO 639 and ISO 3166) names. Prior to Mac OS X 10.3, there is no API for doing this. Therefore we do it ourselves, using a table based on the results of the Mac OS X 10.3.8 function CFLocaleCreateCanonicalLocaleIdentifierFromString(). */ typedef struct { const char legacy[21+1]; const char unixy[5+1]; } legacy_entry; static const legacy_entry legacy_table[] = { { "Afrikaans", "af" }, { "Albanian", "sq" }, { "Amharic", "am" }, { "Arabic", "ar" }, { "Armenian", "hy" }, { "Assamese", "as" }, { "Aymara", "ay" }, { "Azerbaijani", "az" }, { "Basque", "eu" }, { "Belarusian", "be" }, { "Belorussian", "be" }, { "Bengali", "bn" }, { "Brazilian Portugese", "pt_BR" }, { "Brazilian Portuguese", "pt_BR" }, { "Breton", "br" }, { "Bulgarian", "bg" }, { "Burmese", "my" }, { "Byelorussian", "be" }, { "Catalan", "ca" }, { "Chewa", "ny" }, { "Chichewa", "ny" }, { "Chinese", "zh" }, { "Chinese, Simplified", "zh_CN" }, { "Chinese, Traditional", "zh_TW" }, { "Chinese, Tradtional", "zh_TW" }, { "Croatian", "hr" }, { "Czech", "cs" }, { "Danish", "da" }, { "Dutch", "nl" }, { "Dzongkha", "dz" }, { "English", "en" }, { "Esperanto", "eo" }, { "Estonian", "et" }, { "Faroese", "fo" }, { "Farsi", "fa" }, { "Finnish", "fi" }, { "Flemish", "nl_BE" }, { "French", "fr" }, { "Galician", "gl" }, { "Gallegan", "gl" }, { "Georgian", "ka" }, { "German", "de" }, { "Greek", "el" }, { "Greenlandic", "kl" }, { "Guarani", "gn" }, { "Gujarati", "gu" }, { "Hawaiian", "haw" }, /* Yes, "haw", not "cpe". */ { "Hebrew", "he" }, { "Hindi", "hi" }, { "Hungarian", "hu" }, { "Icelandic", "is" }, { "Indonesian", "id" }, { "Inuktitut", "iu" }, { "Irish", "ga" }, { "Italian", "it" }, { "Japanese", "ja" }, { "Javanese", "jv" }, { "Kalaallisut", "kl" }, { "Kannada", "kn" }, { "Kashmiri", "ks" }, { "Kazakh", "kk" }, { "Khmer", "km" }, { "Kinyarwanda", "rw" }, { "Kirghiz", "ky" }, { "Korean", "ko" }, { "Kurdish", "ku" }, { "Latin", "la" }, { "Latvian", "lv" }, { "Lithuanian", "lt" }, { "Macedonian", "mk" }, { "Malagasy", "mg" }, { "Malay", "ms" }, { "Malayalam", "ml" }, { "Maltese", "mt" }, { "Manx", "gv" }, { "Marathi", "mr" }, { "Moldavian", "mo" }, { "Mongolian", "mn" }, { "Nepali", "ne" }, { "Norwegian", "nb" }, /* Yes, "nb", not the obsolete "no". */ { "Nyanja", "ny" }, { "Nynorsk", "nn" }, { "Oriya", "or" }, { "Oromo", "om" }, { "Panjabi", "pa" }, { "Pashto", "ps" }, { "Persian", "fa" }, { "Polish", "pl" }, { "Portuguese", "pt" }, { "Portuguese, Brazilian", "pt_BR" }, { "Punjabi", "pa" }, { "Pushto", "ps" }, { "Quechua", "qu" }, { "Romanian", "ro" }, { "Ruanda", "rw" }, { "Rundi", "rn" }, { "Russian", "ru" }, { "Sami", "se_NO" }, /* Not just "se". */ { "Sanskrit", "sa" }, { "Scottish", "gd" }, { "Serbian", "sr" }, { "Simplified Chinese", "zh_CN" }, { "Sindhi", "sd" }, { "Sinhalese", "si" }, { "Slovak", "sk" }, { "Slovenian", "sl" }, { "Somali", "so" }, { "Spanish", "es" }, { "Sundanese", "su" }, { "Swahili", "sw" }, { "Swedish", "sv" }, { "Tagalog", "tl" }, { "Tajik", "tg" }, { "Tajiki", "tg" }, { "Tamil", "ta" }, { "Tatar", "tt" }, { "Telugu", "te" }, { "Thai", "th" }, { "Tibetan", "bo" }, { "Tigrinya", "ti" }, { "Tongan", "to" }, { "Traditional Chinese", "zh_TW" }, { "Turkish", "tr" }, { "Turkmen", "tk" }, { "Uighur", "ug" }, { "Ukrainian", "uk" }, { "Urdu", "ur" }, { "Uzbek", "uz" }, { "Vietnamese", "vi" }, { "Welsh", "cy" }, { "Yiddish", "yi" } }; /* Convert new-style locale names with language tags (ISO 639 and ISO 15924) to Unix (ISO 639 and ISO 3166) names. */ typedef struct { const char langtag[7+1]; const char unixy[12+1]; } langtag_entry; static const langtag_entry langtag_table[] = { /* Mac OS X has "az-Arab", "az-Cyrl", "az-Latn". The default script for az on Unix is Latin. */ { "az-Latn", "az" }, /* Mac OS X has "ga-dots". Does not yet exist on Unix. */ { "ga-dots", "ga" }, /* Mac OS X has "kk-Cyrl". Does not yet exist on Unix. */ /* Mac OS X has "mn-Cyrl", "mn-Mong". The default script for mn on Unix is Cyrillic. */ { "mn-Cyrl", "mn" }, /* Mac OS X has "ms-Arab", "ms-Latn". The default script for ms on Unix is Latin. */ { "ms-Latn", "ms" }, /* Mac OS X has "tg-Cyrl". The default script for tg on Unix is Cyrillic. */ { "tg-Cyrl", "tg" }, /* Mac OS X has "tk-Cyrl". Does not yet exist on Unix. */ /* Mac OS X has "tt-Cyrl". The default script for tt on Unix is Cyrillic. */ { "tt-Cyrl", "tt" }, /* Mac OS X has "zh-Hans", "zh-Hant". Country codes are used to distinguish these on Unix. */ { "zh-Hans", "zh_CN" }, { "zh-Hant", "zh_TW" } }; /* Convert script names (ISO 15924) to Unix conventions. See http://www.unicode.org/iso15924/iso15924-codes.html */ typedef struct { const char script[4+1]; const char unixy[9+1]; } script_entry; static const script_entry script_table[] = { { "Arab", "arabic" }, { "Cyrl", "cyrillic" }, { "Mong", "mongolian" } }; /* Step 1: Convert using legacy_table. */ if (name[0] >= 'A' && name[0] <= 'Z') { unsigned int i1, i2; i1 = 0; i2 = sizeof (legacy_table) / sizeof (legacy_entry); while (i2 - i1 > 1) { /* At this point we know that if name occurs in legacy_table, its index must be >= i1 and < i2. */ unsigned int i = (i1 + i2) >> 1; const legacy_entry *p = &legacy_table[i]; if (strcmp (name, p->legacy) < 0) i2 = i; else i1 = i; } if (strcmp (name, legacy_table[i1].legacy) == 0) { strcpy (name, legacy_table[i1].unixy); return; } } /* Step 2: Convert using langtag_table and script_table. */ if (strlen (name) == 7 && name[2] == '-') { unsigned int i1, i2; i1 = 0; i2 = sizeof (langtag_table) / sizeof (langtag_entry); while (i2 - i1 > 1) { /* At this point we know that if name occurs in langtag_table, its index must be >= i1 and < i2. */ unsigned int i = (i1 + i2) >> 1; const langtag_entry *p = &langtag_table[i]; if (strcmp (name, p->langtag) < 0) i2 = i; else i1 = i; } if (strcmp (name, langtag_table[i1].langtag) == 0) { strcpy (name, langtag_table[i1].unixy); return; } i1 = 0; i2 = sizeof (script_table) / sizeof (script_entry); while (i2 - i1 > 1) { /* At this point we know that if (name + 3) occurs in script_table, its index must be >= i1 and < i2. */ unsigned int i = (i1 + i2) >> 1; const script_entry *p = &script_table[i]; if (strcmp (name + 3, p->script) < 0) i2 = i; else i1 = i; } if (strcmp (name + 3, script_table[i1].script) == 0) { name[2] = '@'; strcpy (name + 3, script_table[i1].unixy); return; } } /* Step 3: Convert new-style dash to Unix underscore. */ { char *p; for (p = name; *p != '\0'; p++) if (*p == '-') *p = '_'; } } #endif #if defined WINDOWS_NATIVE || defined __CYGWIN__ /* Native Windows or Cygwin */ /* Canonicalize a Windows native locale name to a Unix locale name. NAME is a sufficiently large buffer. On input, it contains the Windows locale name. On output, it contains the Unix locale name. */ # if !defined IN_LIBINTL static # endif void gl_locale_name_canonicalize (char *name) { /* FIXME: This is probably incomplete: it does not handle "zh-Hans" and "zh-Hant". */ char *p; for (p = name; *p != '\0'; p++) if (*p == '-') { *p = '_'; p++; for (; *p != '\0'; p++) { if (*p >= 'a' && *p <= 'z') *p += 'A' - 'a'; if (*p == '-') { *p = '\0'; return; } } return; } } # if !defined IN_LIBINTL static # endif const char * gl_locale_name_from_win32_LANGID (LANGID langid) { /* Activate the new code only when the GETTEXT_MUI environment variable is set, for the time being, since the new code is not well tested. */ if (getenv ("GETTEXT_MUI") != NULL) { static char namebuf[256]; /* Query the system's notion of locale name. On Windows95/98/ME, GetLocaleInfoA returns some incorrect results. But we don't need to support systems that are so old. */ if (GetLocaleInfoA (MAKELCID (langid, SORT_DEFAULT), LOCALE_SNAME, namebuf, sizeof (namebuf) - 1)) { /* Convert it to a Unix locale name. */ gl_locale_name_canonicalize (namebuf); return namebuf; } } /* Internet Explorer has an LCID to RFC3066 name mapping stored in HKEY_CLASSES_ROOT\Mime\Database\Rfc1766. But we better don't use that since IE's i18n subsystem is known to be inconsistent with the native Windows base (e.g. they have different character conversion facilities that produce different results). */ /* Use our own table. */ { int primary, sub; /* Split into language and territory part. */ primary = PRIMARYLANGID (langid); sub = SUBLANGID (langid); /* Dispatch on language. See also http://www.unicode.org/unicode/onlinedat/languages.html . For details about languages, see https://www.ethnologue.com/ . */ switch (primary) { case LANG_AFRIKAANS: switch (sub) { case SUBLANG_AFRIKAANS_SOUTH_AFRICA: return "af_ZA"; } return "af"; case LANG_ALBANIAN: switch (sub) { case SUBLANG_ALBANIAN_ALBANIA: return "sq_AL"; } return "sq"; case LANG_ALSATIAN: switch (sub) { case SUBLANG_ALSATIAN_FRANCE: return "gsw_FR"; } return "gsw"; case LANG_AMHARIC: switch (sub) { case SUBLANG_AMHARIC_ETHIOPIA: return "am_ET"; } return "am"; case LANG_ARABIC: switch (sub) { case SUBLANG_ARABIC_SAUDI_ARABIA: return "ar_SA"; case SUBLANG_ARABIC_IRAQ: return "ar_IQ"; case SUBLANG_ARABIC_EGYPT: return "ar_EG"; case SUBLANG_ARABIC_LIBYA: return "ar_LY"; case SUBLANG_ARABIC_ALGERIA: return "ar_DZ"; case SUBLANG_ARABIC_MOROCCO: return "ar_MA"; case SUBLANG_ARABIC_TUNISIA: return "ar_TN"; case SUBLANG_ARABIC_OMAN: return "ar_OM"; case SUBLANG_ARABIC_YEMEN: return "ar_YE"; case SUBLANG_ARABIC_SYRIA: return "ar_SY"; case SUBLANG_ARABIC_JORDAN: return "ar_JO"; case SUBLANG_ARABIC_LEBANON: return "ar_LB"; case SUBLANG_ARABIC_KUWAIT: return "ar_KW"; case SUBLANG_ARABIC_UAE: return "ar_AE"; case SUBLANG_ARABIC_BAHRAIN: return "ar_BH"; case SUBLANG_ARABIC_QATAR: return "ar_QA"; } return "ar"; case LANG_ARMENIAN: switch (sub) { case SUBLANG_ARMENIAN_ARMENIA: return "hy_AM"; } return "hy"; case LANG_ASSAMESE: switch (sub) { case SUBLANG_ASSAMESE_INDIA: return "as_IN"; } return "as"; case LANG_AZERI: switch (sub) { /* FIXME: Adjust this when Azerbaijani locales appear on Unix. */ case 0x1e: return "az@latin"; case SUBLANG_AZERI_LATIN: return "az_AZ@latin"; case 0x1d: return "az@cyrillic"; case SUBLANG_AZERI_CYRILLIC: return "az_AZ@cyrillic"; } return "az"; case LANG_BASHKIR: switch (sub) { case SUBLANG_BASHKIR_RUSSIA: return "ba_RU"; } return "ba"; case LANG_BASQUE: switch (sub) { case SUBLANG_BASQUE_BASQUE: return "eu_ES"; } return "eu"; /* Ambiguous: could be "eu_ES" or "eu_FR". */ case LANG_BELARUSIAN: switch (sub) { case SUBLANG_BELARUSIAN_BELARUS: return "be_BY"; } return "be"; case LANG_BENGALI: switch (sub) { case SUBLANG_BENGALI_INDIA: return "bn_IN"; case SUBLANG_BENGALI_BANGLADESH: return "bn_BD"; } return "bn"; case LANG_BRETON: switch (sub) { case SUBLANG_BRETON_FRANCE: return "br_FR"; } return "br"; case LANG_BULGARIAN: switch (sub) { case SUBLANG_BULGARIAN_BULGARIA: return "bg_BG"; } return "bg"; case LANG_BURMESE: switch (sub) { case SUBLANG_DEFAULT: return "my_MM"; } return "my"; case LANG_CAMBODIAN: switch (sub) { case SUBLANG_CAMBODIAN_CAMBODIA: return "km_KH"; } return "km"; case LANG_CATALAN: switch (sub) { case SUBLANG_CATALAN_SPAIN: return "ca_ES"; } return "ca"; case LANG_CHEROKEE: switch (sub) { case SUBLANG_DEFAULT: return "chr_US"; } return "chr"; case LANG_CHINESE: switch (sub) { case SUBLANG_CHINESE_TRADITIONAL: case 0x1f: return "zh_TW"; case SUBLANG_CHINESE_SIMPLIFIED: case 0x00: return "zh_CN"; case SUBLANG_CHINESE_HONGKONG: return "zh_HK"; /* traditional */ case SUBLANG_CHINESE_SINGAPORE: return "zh_SG"; /* simplified */ case SUBLANG_CHINESE_MACAU: return "zh_MO"; /* traditional */ } return "zh"; case LANG_CORSICAN: switch (sub) { case SUBLANG_CORSICAN_FRANCE: return "co_FR"; } return "co"; case LANG_CROATIAN: /* LANG_CROATIAN == LANG_SERBIAN == LANG_BOSNIAN * What used to be called Serbo-Croatian * should really now be two separate * languages because of political reasons. * (Says tml, who knows nothing about Serbian * or Croatian.) * (I can feel those flames coming already.) */ switch (sub) { /* Croatian */ case 0x00: return "hr"; case SUBLANG_CROATIAN_CROATIA: return "hr_HR"; case SUBLANG_CROATIAN_BOSNIA_HERZEGOVINA_LATIN: return "hr_BA"; /* Serbian */ case 0x1f: return "sr"; case 0x1c: return "sr"; /* latin */ case SUBLANG_SERBIAN_LATIN: return "sr_CS"; /* latin */ case 0x09: return "sr_RS"; /* latin */ case 0x0b: return "sr_ME"; /* latin */ case 0x06: return "sr_BA"; /* latin */ case 0x1b: return "sr@cyrillic"; case SUBLANG_SERBIAN_CYRILLIC: return "sr_CS@cyrillic"; case 0x0a: return "sr_RS@cyrillic"; case 0x0c: return "sr_ME@cyrillic"; case 0x07: return "sr_BA@cyrillic"; /* Bosnian */ case 0x1e: return "bs"; case 0x1a: return "bs"; /* latin */ case SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_LATIN: return "bs_BA"; /* latin */ case 0x19: return "bs@cyrillic"; case SUBLANG_BOSNIAN_BOSNIA_HERZEGOVINA_CYRILLIC: return "bs_BA@cyrillic"; } return "hr"; case LANG_CZECH: switch (sub) { case SUBLANG_CZECH_CZECH_REPUBLIC: return "cs_CZ"; } return "cs"; case LANG_DANISH: switch (sub) { case SUBLANG_DANISH_DENMARK: return "da_DK"; } return "da"; case LANG_DARI: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_DARI_AFGHANISTAN: return "prs_AF"; } return "prs"; case LANG_DIVEHI: switch (sub) { case SUBLANG_DIVEHI_MALDIVES: return "dv_MV"; } return "dv"; case LANG_DUTCH: switch (sub) { case SUBLANG_DUTCH: return "nl_NL"; case SUBLANG_DUTCH_BELGIAN: /* FLEMISH, VLAAMS */ return "nl_BE"; case SUBLANG_DUTCH_SURINAM: return "nl_SR"; } return "nl"; case LANG_EDO: switch (sub) { case SUBLANG_DEFAULT: return "bin_NG"; } return "bin"; case LANG_ENGLISH: switch (sub) { /* SUBLANG_ENGLISH_US == SUBLANG_DEFAULT. Heh. I thought * English was the language spoken in England. * Oh well. */ case SUBLANG_ENGLISH_US: return "en_US"; case SUBLANG_ENGLISH_UK: return "en_GB"; case SUBLANG_ENGLISH_AUS: return "en_AU"; case SUBLANG_ENGLISH_CAN: return "en_CA"; case SUBLANG_ENGLISH_NZ: return "en_NZ"; case SUBLANG_ENGLISH_EIRE: return "en_IE"; case SUBLANG_ENGLISH_SOUTH_AFRICA: return "en_ZA"; case SUBLANG_ENGLISH_JAMAICA: return "en_JM"; case SUBLANG_ENGLISH_CARIBBEAN: return "en_GD"; /* Grenada? */ case SUBLANG_ENGLISH_BELIZE: return "en_BZ"; case SUBLANG_ENGLISH_TRINIDAD: return "en_TT"; case SUBLANG_ENGLISH_ZIMBABWE: return "en_ZW"; case SUBLANG_ENGLISH_PHILIPPINES: return "en_PH"; case SUBLANG_ENGLISH_INDONESIA: return "en_ID"; case SUBLANG_ENGLISH_HONGKONG: return "en_HK"; case SUBLANG_ENGLISH_INDIA: return "en_IN"; case SUBLANG_ENGLISH_MALAYSIA: return "en_MY"; case SUBLANG_ENGLISH_SINGAPORE: return "en_SG"; } return "en"; case LANG_ESTONIAN: switch (sub) { case SUBLANG_ESTONIAN_ESTONIA: return "et_EE"; } return "et"; case LANG_FAEROESE: switch (sub) { case SUBLANG_FAEROESE_FAROE_ISLANDS: return "fo_FO"; } return "fo"; case LANG_FARSI: switch (sub) { case SUBLANG_FARSI_IRAN: return "fa_IR"; } return "fa"; case LANG_FINNISH: switch (sub) { case SUBLANG_FINNISH_FINLAND: return "fi_FI"; } return "fi"; case LANG_FRENCH: switch (sub) { case SUBLANG_FRENCH: return "fr_FR"; case SUBLANG_FRENCH_BELGIAN: /* WALLOON */ return "fr_BE"; case SUBLANG_FRENCH_CANADIAN: return "fr_CA"; case SUBLANG_FRENCH_SWISS: return "fr_CH"; case SUBLANG_FRENCH_LUXEMBOURG: return "fr_LU"; case SUBLANG_FRENCH_MONACO: return "fr_MC"; case SUBLANG_FRENCH_WESTINDIES: return "fr"; /* Caribbean? */ case SUBLANG_FRENCH_REUNION: return "fr_RE"; case SUBLANG_FRENCH_CONGO: return "fr_CG"; case SUBLANG_FRENCH_SENEGAL: return "fr_SN"; case SUBLANG_FRENCH_CAMEROON: return "fr_CM"; case SUBLANG_FRENCH_COTEDIVOIRE: return "fr_CI"; case SUBLANG_FRENCH_MALI: return "fr_ML"; case SUBLANG_FRENCH_MOROCCO: return "fr_MA"; case SUBLANG_FRENCH_HAITI: return "fr_HT"; } return "fr"; case LANG_FRISIAN: switch (sub) { case SUBLANG_FRISIAN_NETHERLANDS: return "fy_NL"; } return "fy"; case LANG_FULFULDE: /* Spoken in Nigeria, Guinea, Senegal, Mali, Niger, Cameroon, Benin. */ switch (sub) { case SUBLANG_DEFAULT: return "ff_NG"; } return "ff"; case LANG_GAELIC: switch (sub) { case 0x01: /* SCOTTISH */ /* old, superseded by LANG_SCOTTISH_GAELIC */ return "gd_GB"; case SUBLANG_IRISH_IRELAND: return "ga_IE"; } return "ga"; case LANG_GALICIAN: switch (sub) { case SUBLANG_GALICIAN_SPAIN: return "gl_ES"; } return "gl"; case LANG_GEORGIAN: switch (sub) { case SUBLANG_GEORGIAN_GEORGIA: return "ka_GE"; } return "ka"; case LANG_GERMAN: switch (sub) { case SUBLANG_GERMAN: return "de_DE"; case SUBLANG_GERMAN_SWISS: return "de_CH"; case SUBLANG_GERMAN_AUSTRIAN: return "de_AT"; case SUBLANG_GERMAN_LUXEMBOURG: return "de_LU"; case SUBLANG_GERMAN_LIECHTENSTEIN: return "de_LI"; } return "de"; case LANG_GREEK: switch (sub) { case SUBLANG_GREEK_GREECE: return "el_GR"; } return "el"; case LANG_GREENLANDIC: switch (sub) { case SUBLANG_GREENLANDIC_GREENLAND: return "kl_GL"; } return "kl"; case LANG_GUARANI: switch (sub) { case SUBLANG_DEFAULT: return "gn_PY"; } return "gn"; case LANG_GUJARATI: switch (sub) { case SUBLANG_GUJARATI_INDIA: return "gu_IN"; } return "gu"; case LANG_HAUSA: switch (sub) { case 0x1f: return "ha"; case SUBLANG_HAUSA_NIGERIA_LATIN: return "ha_NG"; } return "ha"; case LANG_HAWAIIAN: /* FIXME: Do they mean Hawaiian ("haw_US", 1000 speakers) or Hawaii Creole English ("cpe_US", 600000 speakers)? */ switch (sub) { case SUBLANG_DEFAULT: return "cpe_US"; } return "cpe"; case LANG_HEBREW: switch (sub) { case SUBLANG_HEBREW_ISRAEL: return "he_IL"; } return "he"; case LANG_HINDI: switch (sub) { case SUBLANG_HINDI_INDIA: return "hi_IN"; } return "hi"; case LANG_HUNGARIAN: switch (sub) { case SUBLANG_HUNGARIAN_HUNGARY: return "hu_HU"; } return "hu"; case LANG_IBIBIO: switch (sub) { case SUBLANG_DEFAULT: return "nic_NG"; } return "nic"; case LANG_ICELANDIC: switch (sub) { case SUBLANG_ICELANDIC_ICELAND: return "is_IS"; } return "is"; case LANG_IGBO: switch (sub) { case SUBLANG_IGBO_NIGERIA: return "ig_NG"; } return "ig"; case LANG_INDONESIAN: switch (sub) { case SUBLANG_INDONESIAN_INDONESIA: return "id_ID"; } return "id"; case LANG_INUKTITUT: switch (sub) { case 0x1e: return "iu"; /* syllabic */ case SUBLANG_INUKTITUT_CANADA: return "iu_CA"; /* syllabic */ case 0x1f: return "iu@latin"; case SUBLANG_INUKTITUT_CANADA_LATIN: return "iu_CA@latin"; } return "iu"; case LANG_ITALIAN: switch (sub) { case SUBLANG_ITALIAN: return "it_IT"; case SUBLANG_ITALIAN_SWISS: return "it_CH"; } return "it"; case LANG_JAPANESE: switch (sub) { case SUBLANG_JAPANESE_JAPAN: return "ja_JP"; } return "ja"; case LANG_KANNADA: switch (sub) { case SUBLANG_KANNADA_INDIA: return "kn_IN"; } return "kn"; case LANG_KANURI: switch (sub) { case SUBLANG_DEFAULT: return "kr_NG"; } return "kr"; case LANG_KASHMIRI: switch (sub) { case SUBLANG_DEFAULT: return "ks_PK"; case SUBLANG_KASHMIRI_INDIA: return "ks_IN"; } return "ks"; case LANG_KAZAK: switch (sub) { case SUBLANG_KAZAK_KAZAKHSTAN: return "kk_KZ"; } return "kk"; case LANG_KICHE: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_KICHE_GUATEMALA: return "qut_GT"; } return "qut"; case LANG_KINYARWANDA: switch (sub) { case SUBLANG_KINYARWANDA_RWANDA: return "rw_RW"; } return "rw"; case LANG_KONKANI: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_KONKANI_INDIA: return "kok_IN"; } return "kok"; case LANG_KOREAN: switch (sub) { case SUBLANG_DEFAULT: return "ko_KR"; } return "ko"; case LANG_KYRGYZ: switch (sub) { case SUBLANG_KYRGYZ_KYRGYZSTAN: return "ky_KG"; } return "ky"; case LANG_LAO: switch (sub) { case SUBLANG_LAO_LAOS: return "lo_LA"; } return "lo"; case LANG_LATIN: switch (sub) { case SUBLANG_DEFAULT: return "la_VA"; } return "la"; case LANG_LATVIAN: switch (sub) { case SUBLANG_LATVIAN_LATVIA: return "lv_LV"; } return "lv"; case LANG_LITHUANIAN: switch (sub) { case SUBLANG_LITHUANIAN_LITHUANIA: return "lt_LT"; } return "lt"; case LANG_LUXEMBOURGISH: switch (sub) { case SUBLANG_LUXEMBOURGISH_LUXEMBOURG: return "lb_LU"; } return "lb"; case LANG_MACEDONIAN: switch (sub) { case SUBLANG_MACEDONIAN_MACEDONIA: return "mk_MK"; } return "mk"; case LANG_MALAY: switch (sub) { case SUBLANG_MALAY_MALAYSIA: return "ms_MY"; case SUBLANG_MALAY_BRUNEI_DARUSSALAM: return "ms_BN"; } return "ms"; case LANG_MALAYALAM: switch (sub) { case SUBLANG_MALAYALAM_INDIA: return "ml_IN"; } return "ml"; case LANG_MALTESE: switch (sub) { case SUBLANG_MALTESE_MALTA: return "mt_MT"; } return "mt"; case LANG_MANIPURI: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { case SUBLANG_DEFAULT: return "mni_IN"; } return "mni"; case LANG_MAORI: switch (sub) { case SUBLANG_MAORI_NEW_ZEALAND: return "mi_NZ"; } return "mi"; case LANG_MAPUDUNGUN: switch (sub) { case SUBLANG_MAPUDUNGUN_CHILE: return "arn_CL"; } return "arn"; case LANG_MARATHI: switch (sub) { case SUBLANG_MARATHI_INDIA: return "mr_IN"; } return "mr"; case LANG_MOHAWK: switch (sub) { case SUBLANG_MOHAWK_CANADA: return "moh_CA"; } return "moh"; case LANG_MONGOLIAN: switch (sub) { case SUBLANG_MONGOLIAN_CYRILLIC_MONGOLIA: case 0x1e: return "mn_MN"; case SUBLANG_MONGOLIAN_PRC: case 0x1f: return "mn_CN"; } return "mn"; /* Ambiguous: could be "mn_CN" or "mn_MN". */ case LANG_NEPALI: switch (sub) { case SUBLANG_NEPALI_NEPAL: return "ne_NP"; case SUBLANG_NEPALI_INDIA: return "ne_IN"; } return "ne"; case LANG_NORWEGIAN: switch (sub) { case 0x1f: return "nb"; case SUBLANG_NORWEGIAN_BOKMAL: return "nb_NO"; case 0x1e: return "nn"; case SUBLANG_NORWEGIAN_NYNORSK: return "nn_NO"; } return "no"; case LANG_OCCITAN: switch (sub) { case SUBLANG_OCCITAN_FRANCE: return "oc_FR"; } return "oc"; case LANG_ORIYA: switch (sub) { case SUBLANG_ORIYA_INDIA: return "or_IN"; } return "or"; case LANG_OROMO: switch (sub) { case SUBLANG_DEFAULT: return "om_ET"; } return "om"; case LANG_PAPIAMENTU: switch (sub) { case SUBLANG_DEFAULT: return "pap_AN"; } return "pap"; case LANG_PASHTO: switch (sub) { case SUBLANG_PASHTO_AFGHANISTAN: return "ps_AF"; } return "ps"; /* Ambiguous: could be "ps_PK" or "ps_AF". */ case LANG_POLISH: switch (sub) { case SUBLANG_POLISH_POLAND: return "pl_PL"; } return "pl"; case LANG_PORTUGUESE: switch (sub) { /* Hmm. SUBLANG_PORTUGUESE_BRAZILIAN == SUBLANG_DEFAULT. Same phenomenon as SUBLANG_ENGLISH_US == SUBLANG_DEFAULT. */ case SUBLANG_PORTUGUESE_BRAZILIAN: return "pt_BR"; case SUBLANG_PORTUGUESE: return "pt_PT"; } return "pt"; case LANG_PUNJABI: switch (sub) { case SUBLANG_PUNJABI_INDIA: return "pa_IN"; /* Gurmukhi script */ case SUBLANG_PUNJABI_PAKISTAN: return "pa_PK"; /* Arabic script */ } return "pa"; case LANG_QUECHUA: /* Note: Microsoft uses the non-ISO language code "quz". */ switch (sub) { case SUBLANG_QUECHUA_BOLIVIA: return "qu_BO"; case SUBLANG_QUECHUA_ECUADOR: return "qu_EC"; case SUBLANG_QUECHUA_PERU: return "qu_PE"; } return "qu"; case LANG_ROMANIAN: switch (sub) { case SUBLANG_ROMANIAN_ROMANIA: return "ro_RO"; case SUBLANG_ROMANIAN_MOLDOVA: return "ro_MD"; } return "ro"; case LANG_ROMANSH: switch (sub) { case SUBLANG_ROMANSH_SWITZERLAND: return "rm_CH"; } return "rm"; case LANG_RUSSIAN: switch (sub) { case SUBLANG_RUSSIAN_RUSSIA: return "ru_RU"; case SUBLANG_RUSSIAN_MOLDAVIA: return "ru_MD"; } return "ru"; /* Ambiguous: could be "ru_RU" or "ru_UA" or "ru_MD". */ case LANG_SAMI: switch (sub) { /* Northern Sami */ case 0x00: return "se"; case SUBLANG_SAMI_NORTHERN_NORWAY: return "se_NO"; case SUBLANG_SAMI_NORTHERN_SWEDEN: return "se_SE"; case SUBLANG_SAMI_NORTHERN_FINLAND: return "se_FI"; /* Lule Sami */ case 0x1f: return "smj"; case SUBLANG_SAMI_LULE_NORWAY: return "smj_NO"; case SUBLANG_SAMI_LULE_SWEDEN: return "smj_SE"; /* Southern Sami */ case 0x1e: return "sma"; case SUBLANG_SAMI_SOUTHERN_NORWAY: return "sma_NO"; case SUBLANG_SAMI_SOUTHERN_SWEDEN: return "sma_SE"; /* Skolt Sami */ case 0x1d: return "sms"; case SUBLANG_SAMI_SKOLT_FINLAND: return "sms_FI"; /* Inari Sami */ case 0x1c: return "smn"; case SUBLANG_SAMI_INARI_FINLAND: return "smn_FI"; } return "se"; /* or "smi"? */ case LANG_SANSKRIT: switch (sub) { case SUBLANG_SANSKRIT_INDIA: return "sa_IN"; } return "sa"; case LANG_SCOTTISH_GAELIC: switch (sub) { case SUBLANG_DEFAULT: return "gd_GB"; } return "gd"; case LANG_SINDHI: switch (sub) { case SUBLANG_SINDHI_INDIA: return "sd_IN"; case SUBLANG_SINDHI_PAKISTAN: return "sd_PK"; /*case SUBLANG_SINDHI_AFGHANISTAN: return "sd_AF";*/ } return "sd"; case LANG_SINHALESE: switch (sub) { case SUBLANG_SINHALESE_SRI_LANKA: return "si_LK"; } return "si"; case LANG_SLOVAK: switch (sub) { case SUBLANG_SLOVAK_SLOVAKIA: return "sk_SK"; } return "sk"; case LANG_SLOVENIAN: switch (sub) { case SUBLANG_SLOVENIAN_SLOVENIA: return "sl_SI"; } return "sl"; case LANG_SOMALI: switch (sub) { case SUBLANG_DEFAULT: return "so_SO"; } return "so"; case LANG_SORBIAN: /* FIXME: Adjust this when such locales appear on Unix. */ switch (sub) { /* Upper Sorbian */ case 0x00: return "hsb"; case SUBLANG_UPPER_SORBIAN_GERMANY: return "hsb_DE"; /* Lower Sorbian */ case 0x1f: return "dsb"; case SUBLANG_LOWER_SORBIAN_GERMANY: return "dsb_DE"; } return "wen"; case LANG_SOTHO: /* calls it "Sesotho sa Leboa"; according to it's the same as Northern Sotho. */ switch (sub) { case SUBLANG_SOTHO_SOUTH_AFRICA: return "nso_ZA"; } return "nso"; case LANG_SPANISH: switch (sub) { case SUBLANG_SPANISH: return "es_ES"; case SUBLANG_SPANISH_MEXICAN: return "es_MX"; case SUBLANG_SPANISH_MODERN: return "es_ES@modern"; /* not seen on Unix */ case SUBLANG_SPANISH_GUATEMALA: return "es_GT"; case SUBLANG_SPANISH_COSTA_RICA: return "es_CR"; case SUBLANG_SPANISH_PANAMA: return "es_PA"; case SUBLANG_SPANISH_DOMINICAN_REPUBLIC: return "es_DO"; case SUBLANG_SPANISH_VENEZUELA: return "es_VE"; case SUBLANG_SPANISH_COLOMBIA: return "es_CO"; case SUBLANG_SPANISH_PERU: return "es_PE"; case SUBLANG_SPANISH_ARGENTINA: return "es_AR"; case SUBLANG_SPANISH_ECUADOR: return "es_EC"; case SUBLANG_SPANISH_CHILE: return "es_CL"; case SUBLANG_SPANISH_URUGUAY: return "es_UY"; case SUBLANG_SPANISH_PARAGUAY: return "es_PY"; case SUBLANG_SPANISH_BOLIVIA: return "es_BO"; case SUBLANG_SPANISH_EL_SALVADOR: return "es_SV"; case SUBLANG_SPANISH_HONDURAS: return "es_HN"; case SUBLANG_SPANISH_NICARAGUA: return "es_NI"; case SUBLANG_SPANISH_PUERTO_RICO: return "es_PR"; case SUBLANG_SPANISH_US: return "es_US"; } return "es"; case LANG_SUTU: switch (sub) { case SUBLANG_DEFAULT: return "bnt_TZ"; /* or "st_LS" or "nso_ZA"? */ } return "bnt"; case LANG_SWAHILI: switch (sub) { case SUBLANG_SWAHILI_KENYA: return "sw_KE"; } return "sw"; case LANG_SWEDISH: switch (sub) { case SUBLANG_SWEDISH_SWEDEN: return "sv_SE"; case SUBLANG_SWEDISH_FINLAND: return "sv_FI"; } return "sv"; case LANG_SYRIAC: switch (sub) { case SUBLANG_SYRIAC_SYRIA: return "syr_SY"; /* An extinct language. */ } return "syr"; case LANG_TAGALOG: switch (sub) { case SUBLANG_TAGALOG_PHILIPPINES: return "tl_PH"; /* or "fil_PH"? */ } return "tl"; /* or "fil"? */ case LANG_TAJIK: switch (sub) { case 0x1f: return "tg"; case SUBLANG_TAJIK_TAJIKISTAN: return "tg_TJ"; } return "tg"; case LANG_TAMAZIGHT: /* Note: Microsoft uses the non-ISO language code "tmz". */ switch (sub) { /* FIXME: Adjust this when Tamazight locales appear on Unix. */ case SUBLANG_TAMAZIGHT_ARABIC: return "ber_MA@arabic"; case 0x1f: return "ber@latin"; case SUBLANG_TAMAZIGHT_ALGERIA_LATIN: return "ber_DZ@latin"; } return "ber"; case LANG_TAMIL: switch (sub) { case SUBLANG_TAMIL_INDIA: return "ta_IN"; } return "ta"; /* Ambiguous: could be "ta_IN" or "ta_LK" or "ta_SG". */ case LANG_TATAR: switch (sub) { case SUBLANG_TATAR_RUSSIA: return "tt_RU"; } return "tt"; case LANG_TELUGU: switch (sub) { case SUBLANG_TELUGU_INDIA: return "te_IN"; } return "te"; case LANG_THAI: switch (sub) { case SUBLANG_THAI_THAILAND: return "th_TH"; } return "th"; case LANG_TIBETAN: switch (sub) { case SUBLANG_TIBETAN_PRC: /* Most Tibetans would not like "bo_CN". But Tibet does not yet have a country code of its own. */ return "bo"; case SUBLANG_TIBETAN_BHUTAN: return "bo_BT"; } return "bo"; case LANG_TIGRINYA: switch (sub) { case SUBLANG_TIGRINYA_ETHIOPIA: return "ti_ET"; case SUBLANG_TIGRINYA_ERITREA: return "ti_ER"; } return "ti"; case LANG_TSONGA: switch (sub) { case SUBLANG_DEFAULT: return "ts_ZA"; } return "ts"; case LANG_TSWANA: /* Spoken in South Africa, Botswana. */ switch (sub) { case SUBLANG_TSWANA_SOUTH_AFRICA: return "tn_ZA"; } return "tn"; case LANG_TURKISH: switch (sub) { case SUBLANG_TURKISH_TURKEY: return "tr_TR"; } return "tr"; case LANG_TURKMEN: switch (sub) { case SUBLANG_TURKMEN_TURKMENISTAN: return "tk_TM"; } return "tk"; case LANG_UIGHUR: switch (sub) { case SUBLANG_UIGHUR_PRC: return "ug_CN"; } return "ug"; case LANG_UKRAINIAN: switch (sub) { case SUBLANG_UKRAINIAN_UKRAINE: return "uk_UA"; } return "uk"; case LANG_URDU: switch (sub) { case SUBLANG_URDU_PAKISTAN: return "ur_PK"; case SUBLANG_URDU_INDIA: return "ur_IN"; } return "ur"; case LANG_UZBEK: switch (sub) { case 0x1f: return "uz"; case SUBLANG_UZBEK_LATIN: return "uz_UZ"; case 0x1e: return "uz@cyrillic"; case SUBLANG_UZBEK_CYRILLIC: return "uz_UZ@cyrillic"; } return "uz"; case LANG_VENDA: switch (sub) { case SUBLANG_DEFAULT: return "ve_ZA"; } return "ve"; case LANG_VIETNAMESE: switch (sub) { case SUBLANG_VIETNAMESE_VIETNAM: return "vi_VN"; } return "vi"; case LANG_WELSH: switch (sub) { case SUBLANG_WELSH_UNITED_KINGDOM: return "cy_GB"; } return "cy"; case LANG_WOLOF: switch (sub) { case SUBLANG_WOLOF_SENEGAL: return "wo_SN"; } return "wo"; case LANG_XHOSA: switch (sub) { case SUBLANG_XHOSA_SOUTH_AFRICA: return "xh_ZA"; } return "xh"; case LANG_YAKUT: switch (sub) { case SUBLANG_YAKUT_RUSSIA: return "sah_RU"; } return "sah"; case LANG_YI: switch (sub) { case SUBLANG_YI_PRC: return "ii_CN"; } return "ii"; case LANG_YIDDISH: switch (sub) { case SUBLANG_DEFAULT: return "yi_IL"; } return "yi"; case LANG_YORUBA: switch (sub) { case SUBLANG_YORUBA_NIGERIA: return "yo_NG"; } return "yo"; case LANG_ZULU: switch (sub) { case SUBLANG_ZULU_SOUTH_AFRICA: return "zu_ZA"; } return "zu"; default: return "C"; } } } # if !defined IN_LIBINTL static # endif const char * gl_locale_name_from_win32_LCID (LCID lcid) { LANGID langid; /* Strip off the sorting rules, keep only the language part. */ langid = LANGIDFROMLCID (lcid); return gl_locale_name_from_win32_LANGID (langid); } # ifdef WINDOWS_NATIVE /* Two variables to interface between get_lcid and the EnumLocales callback function below. */ static LCID found_lcid; static char lname[LC_MAX * (LOCALE_NAME_MAX_LENGTH + 1) + 1]; /* Callback function for EnumLocales. */ static BOOL CALLBACK enum_locales_fn (LPTSTR locale_num_str) { char *endp; char locval[2 * LOCALE_NAME_MAX_LENGTH + 1 + 1]; LCID try_lcid = strtoul (locale_num_str, &endp, 16); if (GetLocaleInfo (try_lcid, LOCALE_SENGLANGUAGE, locval, LOCALE_NAME_MAX_LENGTH)) { strcat (locval, "_"); if (GetLocaleInfo (try_lcid, LOCALE_SENGCOUNTRY, locval + strlen (locval), LOCALE_NAME_MAX_LENGTH)) { size_t locval_len = strlen (locval); if (strncmp (locval, lname, locval_len) == 0 && (lname[locval_len] == '.' || lname[locval_len] == '\0')) { found_lcid = try_lcid; return FALSE; } } } return TRUE; } /* This lock protects the get_lcid against multiple simultaneous calls. */ gl_lock_define_initialized(static, get_lcid_lock) /* Return the Locale ID (LCID) number given the locale's name, a string, in LOCALE_NAME. This works by enumerating all the locales supported by the system, until we find one whose name matches LOCALE_NAME. */ static LCID get_lcid (const char *locale_name) { /* A simple cache. */ static LCID last_lcid; static char last_locale[1000]; /* Lock while looking for an LCID, to protect access to static variables: last_lcid, last_locale, found_lcid, and lname. */ gl_lock_lock (get_lcid_lock); if (last_lcid > 0 && strcmp (locale_name, last_locale) == 0) { gl_lock_unlock (get_lcid_lock); return last_lcid; } strncpy (lname, locale_name, sizeof (lname) - 1); lname[sizeof (lname) - 1] = '\0'; found_lcid = 0; EnumSystemLocales (enum_locales_fn, LCID_SUPPORTED); if (found_lcid > 0) { last_lcid = found_lcid; strcpy (last_locale, locale_name); } gl_lock_unlock (get_lcid_lock); return found_lcid; } # endif #endif #if HAVE_USELOCALE /* glibc, Solaris >= 12 or Mac OS X */ /* Simple hash set of strings. We don't want to drag in lots of hash table code here. */ # define SIZE_BITS (sizeof (size_t) * CHAR_BIT) /* A hash function for NUL-terminated char* strings using the method described by Bruno Haible. See https://www.haible.de/bruno/hashfunc.html. */ static size_t _GL_ATTRIBUTE_PURE string_hash (const void *x) { const char *s = (const char *) x; size_t h = 0; for (; *s; s++) h = *s + ((h << 9) | (h >> (SIZE_BITS - 9))); return h; } /* A hash table of fixed size. Multiple threads can access it read-only simultaneously, but only one thread can insert into it at the same time. */ /* A node in a hash bucket collision list. */ struct hash_node { struct hash_node * volatile next; char contents[FLEXIBLE_ARRAY_MEMBER]; }; # define HASH_TABLE_SIZE 257 static struct hash_node * volatile struniq_hash_table[HASH_TABLE_SIZE] /* = { NULL, ..., NULL } */; /* This lock protects the struniq_hash_table against multiple simultaneous insertions. */ gl_lock_define_initialized(static, struniq_lock) /* Store a copy of the given string in a string pool with indefinite extent. Return a pointer to this copy. */ static const char * struniq (const char *string) { size_t hashcode = string_hash (string); size_t slot = hashcode % HASH_TABLE_SIZE; size_t size; struct hash_node *new_node; struct hash_node *p; for (p = struniq_hash_table[slot]; p != NULL; p = p->next) if (strcmp (p->contents, string) == 0) return p->contents; size = strlen (string) + 1; new_node = (struct hash_node *) malloc (FLEXSIZEOF (struct hash_node, contents, size)); if (new_node == NULL) /* Out of memory. Return a statically allocated string. */ return "C"; memcpy (new_node->contents, string, size); /* Lock while inserting new_node. */ gl_lock_lock (struniq_lock); /* Check whether another thread already added the string while we were waiting on the lock. */ for (p = struniq_hash_table[slot]; p != NULL; p = p->next) if (strcmp (p->contents, string) == 0) { free (new_node); new_node = p; goto done; } /* Really insert new_node into the hash table. Fill new_node entirely first, because other threads may be iterating over the linked list. */ new_node->next = struniq_hash_table[slot]; struniq_hash_table[slot] = new_node; done: /* Unlock after new_node is inserted. */ gl_lock_unlock (struniq_lock); return new_node->contents; } #endif #if defined IN_LIBINTL || HAVE_USELOCALE /* Like gl_locale_name_thread, except that the result is not in storage of indefinite extent. */ # if !defined IN_LIBINTL static # endif const char * gl_locale_name_thread_unsafe (int category, const char *categoryname) { # if HAVE_USELOCALE { locale_t thread_locale = uselocale (NULL); if (thread_locale != LC_GLOBAL_LOCALE) { # if __GLIBC__ >= 2 && !defined __UCLIBC__ /* Work around an incorrect definition of the _NL_LOCALE_NAME macro in glibc < 2.12. See . */ const char *name = nl_langinfo (_NL_ITEM ((category), _NL_ITEM_INDEX (-1))); if (name[0] == '\0') /* Fallback code for glibc < 2.4, which did not implement nl_langinfo (_NL_LOCALE_NAME (category)). */ name = thread_locale->__names[category]; return name; # elif (defined __FreeBSD__ || defined __DragonFly__) || (defined __APPLE__ && defined __MACH__) /* FreeBSD, Mac OS X */ int mask; switch (category) { case LC_CTYPE: mask = LC_CTYPE_MASK; break; case LC_NUMERIC: mask = LC_NUMERIC_MASK; break; case LC_TIME: mask = LC_TIME_MASK; break; case LC_COLLATE: mask = LC_COLLATE_MASK; break; case LC_MONETARY: mask = LC_MONETARY_MASK; break; case LC_MESSAGES: mask = LC_MESSAGES_MASK; break; default: /* We shouldn't get here. */ return ""; } return querylocale (mask, thread_locale); # elif defined __sun && HAVE_GETLOCALENAME_L /* Solaris >= 12. */ return getlocalename_l (category, thread_locale); # elif defined __CYGWIN__ /* Cygwin < 2.6 lacks uselocale and thread-local locales altogether. Cygwin <= 2.6.1 lacks NL_LOCALE_NAME, requiring peeking inside an opaque struct. */ # ifdef NL_LOCALE_NAME return nl_langinfo_l (NL_LOCALE_NAME (category), thread_locale); # else /* FIXME: Remove when we can assume new-enough Cygwin. */ struct __locale_t { char categories[7][32]; }; return ((struct __locale_t *) thread_locale)->categories[category]; # endif # elif defined __ANDROID__ return MB_CUR_MAX == 4 ? "C.UTF-8" : "C"; # endif } } # endif return NULL; } #endif const char * gl_locale_name_thread (int category, const char *categoryname) { #if HAVE_USELOCALE const char *name = gl_locale_name_thread_unsafe (category, categoryname); if (name != NULL) return struniq (name); #elif defined WINDOWS_NATIVE if (LC_MIN <= category && category <= LC_MAX) { char *locname = setlocale (category, NULL); LCID lcid = 0; /* If CATEGORY is LC_ALL, the result might be a semi-colon separated list of locales. We need only one, so we take the one corresponding to LC_CTYPE, as the most important for character translations. */ if (strchr (locname, ';')) locname = setlocale (LC_CTYPE, NULL); /* Convert locale name to LCID. We don't want to use LocaleNameToLCID because (a) it is only available since Vista, and (b) it doesn't accept locale names returned by 'setlocale'. */ lcid = get_lcid (locname); if (lcid > 0) return gl_locale_name_from_win32_LCID (lcid); } #endif return NULL; } /* XPG3 defines the result of 'setlocale (category, NULL)' as: "Directs 'setlocale()' to query 'category' and return the current setting of 'local'." However it does not specify the exact format. Neither do SUSV2 and ISO C 99. So we can use this feature only on selected systems (e.g. those using GNU C Library). */ #if defined _LIBC || ((defined __GLIBC__ && __GLIBC__ >= 2) && !defined __UCLIBC__) # define HAVE_LOCALE_NULL #endif const char * gl_locale_name_posix (int category, const char *categoryname) { /* Use the POSIX methods of looking to 'LC_ALL', 'LC_xxx', and 'LANG'. On some systems this can be done by the 'setlocale' function itself. */ #if defined HAVE_SETLOCALE && defined HAVE_LC_MESSAGES && defined HAVE_LOCALE_NULL return setlocale (category, NULL); #else /* On other systems we ignore what setlocale reports and instead look at the environment variables directly. This is necessary 1. on systems which have a facility for customizing the default locale (Mac OS X, native Windows, Cygwin) and where the system's setlocale() function ignores this default locale (Mac OS X, Cygwin), in two cases: a. when the user missed to use the setlocale() override from libintl (for example by not including ), b. when setlocale supports only the "C" locale, such as on Cygwin 1.5.x. In this case even the override from libintl cannot help. 2. on all systems where setlocale supports only the "C" locale. */ /* Strictly speaking, it is a POSIX violation to look at the environment variables regardless whether setlocale has been called or not. POSIX says: "For C-language programs, the POSIX locale shall be the default locale when the setlocale() function is not called." But we assume that all programs that use internationalized APIs call setlocale (LC_ALL, ""). */ return gl_locale_name_environ (category, categoryname); #endif } const char * gl_locale_name_environ (int category, const char *categoryname) { const char *retval; /* Setting of LC_ALL overrides all other. */ retval = getenv ("LC_ALL"); if (retval != NULL && retval[0] != '\0') return retval; /* Next comes the name of the desired category. */ retval = getenv (categoryname); if (retval != NULL && retval[0] != '\0') return retval; /* Last possibility is the LANG environment variable. */ retval = getenv ("LANG"); if (retval != NULL && retval[0] != '\0') { #if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer. Ignore invalid LANG value set by the Terminal application. */ if (strcmp (retval, "UTF-8") != 0) #endif #if defined __CYGWIN__ /* Cygwin. Ignore dummy LANG value set by ~/.profile. */ if (strcmp (retval, "C.UTF-8") != 0) #endif return retval; } return NULL; } const char * gl_locale_name_default (void) { /* POSIX:2001 says: "All implementations shall define a locale as the default locale, to be invoked when no environment variables are set, or set to the empty string. This default locale can be the POSIX locale or any other implementation-defined locale. Some implementations may provide facilities for local installation administrators to set the default locale, customizing it for each location. POSIX:2001 does not require such a facility. The systems with such a facility are Mac OS X and Windows: They provide a GUI that allows the user to choose a locale. - On Mac OS X, by default, none of LC_* or LANG are set. Starting with Mac OS X 10.4 or 10.5, LANG is set for processes launched by the 'Terminal' application (but sometimes to an incorrect value "UTF-8"). When no environment variable is set, setlocale (LC_ALL, "") uses the "C" locale. - On native Windows, by default, none of LC_* or LANG are set. When no environment variable is set, setlocale (LC_ALL, "") uses the locale chosen by the user. - On Cygwin 1.5.x, by default, none of LC_* or LANG are set. When no environment variable is set, setlocale (LC_ALL, "") uses the "C" locale. - On Cygwin 1.7, by default, LANG is set to "C.UTF-8" when the default ~/.profile is executed. When no environment variable is set, setlocale (LC_ALL, "") uses the "C.UTF-8" locale, which operates in the same way as the "C" locale. */ #if !(HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE || defined WINDOWS_NATIVE || defined __CYGWIN__) /* The system does not have a way of setting the locale, other than the POSIX specified environment variables. We use C as default locale. */ return "C"; #else /* Return an XPG style locale name language[_territory][@modifier]. Don't even bother determining the codeset; it's not useful in this context, because message catalogs are not specific to a single codeset. */ # if HAVE_CFLOCALECOPYCURRENT || HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer */ { /* Cache the locale name, since CoreFoundation calls are expensive. */ static const char *cached_localename; if (cached_localename == NULL) { char namebuf[256]; # if HAVE_CFLOCALECOPYCURRENT /* Mac OS X 10.3 or newer */ CFLocaleRef locale = CFLocaleCopyCurrent (); CFStringRef name = CFLocaleGetIdentifier (locale); if (CFStringGetCString (name, namebuf, sizeof (namebuf), kCFStringEncodingASCII)) { gl_locale_name_canonicalize (namebuf); cached_localename = strdup (namebuf); } CFRelease (locale); # elif HAVE_CFPREFERENCESCOPYAPPVALUE /* Mac OS X 10.2 or newer */ CFTypeRef value = CFPreferencesCopyAppValue (CFSTR ("AppleLocale"), kCFPreferencesCurrentApplication); if (value != NULL && CFGetTypeID (value) == CFStringGetTypeID () && CFStringGetCString ((CFStringRef)value, namebuf, sizeof (namebuf), kCFStringEncodingASCII)) { gl_locale_name_canonicalize (namebuf); cached_localename = strdup (namebuf); } # endif if (cached_localename == NULL) cached_localename = "C"; } return cached_localename; } # endif # if defined WINDOWS_NATIVE || defined __CYGWIN__ /* Native Windows or Cygwin */ { LCID lcid; /* Use native Windows API locale ID. */ lcid = GetThreadLocale (); return gl_locale_name_from_win32_LCID (lcid); } # endif #endif } /* Determine the current locale's name, and canonicalize it into XPG syntax language[_territory][.codeset][@modifier] The codeset part in the result is not reliable; the locale_charset() should be used for codeset information instead. The result must not be freed; it is statically allocated. */ const char * gl_locale_name (int category, const char *categoryname) { const char *retval; retval = gl_locale_name_thread (category, categoryname); if (retval != NULL) return retval; retval = gl_locale_name_posix (category, categoryname); if (retval != NULL) return retval; return gl_locale_name_default (); } gnuastro-0.5/bootstrapped/tests/fd-hook.c0000644000175000017500000000700413217200022015472 00000000000000/* Hook for making file descriptor functions close(), ioctl() extensible. Copyright (C) 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2009. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include "fd-hook.h" #include /* Currently, this entire code is only needed for the handling of sockets on native Windows platforms. */ #if WINDOWS_SOCKETS /* The first and last link in the doubly linked list. Initially the list is empty. */ static struct fd_hook anchor = { &anchor, &anchor, NULL, NULL }; int execute_close_hooks (const struct fd_hook *remaining_list, gl_close_fn primary, int fd) { if (remaining_list == &anchor) /* End of list reached. */ return primary (fd); else return remaining_list->private_close_fn (remaining_list->private_next, primary, fd); } int execute_all_close_hooks (gl_close_fn primary, int fd) { return execute_close_hooks (anchor.private_next, primary, fd); } int execute_ioctl_hooks (const struct fd_hook *remaining_list, gl_ioctl_fn primary, int fd, int request, void *arg) { if (remaining_list == &anchor) /* End of list reached. */ return primary (fd, request, arg); else return remaining_list->private_ioctl_fn (remaining_list->private_next, primary, fd, request, arg); } int execute_all_ioctl_hooks (gl_ioctl_fn primary, int fd, int request, void *arg) { return execute_ioctl_hooks (anchor.private_next, primary, fd, request, arg); } void register_fd_hook (close_hook_fn close_hook, ioctl_hook_fn ioctl_hook, struct fd_hook *link) { if (close_hook == NULL) close_hook = execute_close_hooks; if (ioctl_hook == NULL) ioctl_hook = execute_ioctl_hooks; if (link->private_next == NULL && link->private_prev == NULL) { /* Add the link to the doubly linked list. */ link->private_next = anchor.private_next; link->private_prev = &anchor; link->private_close_fn = close_hook; link->private_ioctl_fn = ioctl_hook; anchor.private_next->private_prev = link; anchor.private_next = link; } else { /* The link is already in use. */ if (link->private_close_fn != close_hook || link->private_ioctl_fn != ioctl_hook) abort (); } } void unregister_fd_hook (struct fd_hook *link) { struct fd_hook *next = link->private_next; struct fd_hook *prev = link->private_prev; if (next != NULL && prev != NULL) { /* The link is in use. Remove it from the doubly linked list. */ prev->private_next = next; next->private_prev = prev; /* Clear the link, to mark it unused. */ link->private_next = NULL; link->private_prev = NULL; link->private_close_fn = NULL; link->private_ioctl_fn = NULL; } } #endif gnuastro-0.5/bootstrapped/tests/cloexec.c0000644000175000017500000000442713217200022015573 00000000000000/* cloexec.c - set or clear the close-on-exec descriptor flag Copyright (C) 1991, 2004-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . The code is taken from glibc/manual/llio.texi */ #include #include "cloexec.h" #include #include #include /* Set the 'FD_CLOEXEC' flag of DESC if VALUE is true, or clear the flag if VALUE is false. Return 0 on success, or -1 on error with 'errno' set. Note that on MingW, this function does NOT protect DESC from being inherited into spawned children. Instead, either use dup_cloexec followed by closing the original DESC, or use interfaces such as open or pipe2 that accept flags like O_CLOEXEC to create DESC non-inheritable in the first place. */ int set_cloexec_flag (int desc, bool value) { #ifdef F_SETFD int flags = fcntl (desc, F_GETFD, 0); if (0 <= flags) { int newflags = (value ? flags | FD_CLOEXEC : flags & ~FD_CLOEXEC); if (flags == newflags || fcntl (desc, F_SETFD, newflags) != -1) return 0; } return -1; #else /* !F_SETFD */ /* Use dup2 to reject invalid file descriptors; the cloexec flag will be unaffected. */ if (desc < 0) { errno = EBADF; return -1; } if (dup2 (desc, desc) < 0) /* errno is EBADF here. */ return -1; /* There is nothing we can do on this kind of platform. Punt. */ return 0; #endif /* !F_SETFD */ } /* Duplicates a file handle FD, while marking the copy to be closed prior to exec or spawn. Returns -1 and sets errno if FD could not be duplicated. */ int dup_cloexec (int fd) { return fcntl (fd, F_DUPFD_CLOEXEC, 0); } gnuastro-0.5/bootstrapped/tests/c-strncasecmp.c0000644000175000017500000000310713217200022016705 00000000000000/* c-strncasecmp.c -- case insensitive string comparator in C locale Copyright (C) 1998-1999, 2005-2006, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "c-strcase.h" #include #include "c-ctype.h" int c_strncasecmp (const char *s1, const char *s2, size_t n) { register const unsigned char *p1 = (const unsigned char *) s1; register const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2 || n == 0) return 0; do { c1 = c_tolower (*p1); c2 = c_tolower (*p2); if (--n == 0 || c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.5/bootstrapped/tests/c-strcasecmp.c0000644000175000017500000000304513217200022016530 00000000000000/* c-strcasecmp.c -- case insensitive string comparator in C locale Copyright (C) 1998-1999, 2005-2006, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "c-strcase.h" #include #include "c-ctype.h" int c_strcasecmp (const char *s1, const char *s2) { register const unsigned char *p1 = (const unsigned char *) s1; register const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2) return 0; do { c1 = c_tolower (*p1); c2 = c_tolower (*p2); if (c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.5/bootstrapped/tests/c-strcase.h0000644000175000017500000000401513217200022016033 00000000000000/* Case-insensitive string comparison functions in C locale. Copyright (C) 1995-1996, 2001, 2003, 2005, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef C_STRCASE_H #define C_STRCASE_H #include /* The functions defined in this file assume the "C" locale and a character set without diacritics (ASCII-US or EBCDIC-US or something like that). Even if the "C" locale on a particular system is an extension of the ASCII character set (like on BeOS, where it is UTF-8, or on AmigaOS, where it is ISO-8859-1), the functions in this file recognize only the ASCII characters. More precisely, one of the string arguments must be an ASCII string; the other one can also contain non-ASCII characters (but then the comparison result will be nonzero). */ #ifdef __cplusplus extern "C" { #endif /* Compare strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. */ extern int c_strcasecmp (const char *s1, const char *s2) _GL_ATTRIBUTE_PURE; /* Compare no more than N characters of strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. */ extern int c_strncasecmp (const char *s1, const char *s2, size_t n) _GL_ATTRIBUTE_PURE; #ifdef __cplusplus } #endif #endif /* C_STRCASE_H */ gnuastro-0.5/bootstrapped/tests/binary-io.c0000644000175000017500000000177713217200022016047 00000000000000/* Binary mode I/O. Copyright 2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #define BINARY_IO_INLINE _GL_EXTERN_INLINE #include "binary-io.h" #if defined __DJGPP__ || defined __EMX__ # include # include int __gl_setmode_check (int fd) { if (isatty (fd)) { errno = EINVAL; return -1; } else return 0; } #endif gnuastro-0.5/bootstrapped/tests/binary-io.h0000644000175000017500000000474713217200022016054 00000000000000/* Binary mode I/O. Copyright (C) 2001, 2003, 2005, 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _BINARY_H #define _BINARY_H /* For systems that distinguish between text and binary I/O. O_BINARY is guaranteed by the gnulib . */ #include /* The MSVC7 doesn't like to be included after '#define fileno ...', so we include it here first. */ #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef BINARY_IO_INLINE # define BINARY_IO_INLINE _GL_INLINE #endif #if O_BINARY # if defined __EMX__ || defined __DJGPP__ || defined __CYGWIN__ # include /* declares setmode() */ # define __gl_setmode setmode # else # define __gl_setmode _setmode # undef fileno # define fileno _fileno # endif #else /* On reasonable systems, binary I/O is the only choice. */ /* Use a function rather than a macro, to avoid gcc warnings "warning: statement with no effect". */ BINARY_IO_INLINE int __gl_setmode (int fd, int mode) { (void) fd; (void) mode; return O_BINARY; } #endif #if defined __DJGPP__ || defined __EMX__ extern int __gl_setmode_check (int); #else BINARY_IO_INLINE int __gl_setmode_check (int fd) { return 0; } #endif /* Set FD's mode to MODE, which should be either O_TEXT or O_BINARY. Return the old mode if successful, -1 (setting errno) on failure. Ordinarily this function would be called 'setmode', since that is its name on MS-Windows, but it is called 'set_binary_mode' here to avoid colliding with a BSD function of another name. */ BINARY_IO_INLINE int set_binary_mode (int fd, int mode) { int r = __gl_setmode_check (fd); return r != 0 ? r : __gl_setmode (fd, mode); } /* This macro is obsolescent. */ #define SET_BINARY(fd) ((void) set_binary_mode (fd, O_BINARY)) _GL_INLINE_HEADER_END #endif /* _BINARY_H */ gnuastro-0.5/bootstrapped/tests/Makefile.in0000644000175000017500000074142213217217706016076 00000000000000# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ # Copyright (C) 2002-2017 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; \ elif test -n '$(MAKE_HOST)'; then \ true; \ elif test -n '$(MAKE_VERSION)' && test -n '$(CURDIR)'; then \ true; \ else \ false; \ fi; \ } am__make_running_with_option = \ case $${target_option-} in \ ?) ;; \ *) echo "am__make_running_with_option: internal error: invalid" \ "target option '$${target_option-}' specified" >&2; \ exit 1;; \ esac; \ has_opt=no; \ sane_makeflags=$$MAKEFLAGS; \ if $(am__is_gnu_make); then \ sane_makeflags=$$MFLAGS; \ else \ case $$MAKEFLAGS in \ *\\[\ \ ]*) \ bs=\\; \ sane_makeflags=`printf '%s\n' "$$MAKEFLAGS" \ | sed "s/$$bs$$bs[$$bs $$bs ]*//g"`;; \ esac; \ fi; \ skip_next=no; \ strip_trailopt () \ { \ flg=`printf '%s\n' "$$flg" | sed "s/$$1.*$$//"`; \ }; \ for flg in $$sane_makeflags; do \ test $$skip_next = yes && { skip_next=no; continue; }; \ case $$flg in \ *=*|--*) continue;; \ -*I) strip_trailopt 'I'; skip_next=yes;; \ -*I?*) strip_trailopt 'I';; \ -*O) strip_trailopt 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test-argp$(EXEEXT) test-argp-2.sh test-arpa_inet$(EXEEXT) \ test-binary-io.sh test-bind$(EXEEXT) test-btowc1.sh \ test-btowc2.sh test-c-ctype$(EXEEXT) test-c-strcase.sh \ test-cloexec$(EXEEXT) test-close$(EXEEXT) \ test-connect$(EXEEXT) test-ctype$(EXEEXT) test-dup2$(EXEEXT) \ test-environ$(EXEEXT) test-errno$(EXEEXT) \ test-fcntl-h$(EXEEXT) test-fcntl$(EXEEXT) test-fdopen$(EXEEXT) \ test-fgetc$(EXEEXT) test-float$(EXEEXT) test-fputc$(EXEEXT) \ test-fread$(EXEEXT) test-fstat$(EXEEXT) test-ftruncate.sh \ test-func$(EXEEXT) test-fwrite$(EXEEXT) \ test-getcwd-lgpl$(EXEEXT) test-getdelim$(EXEEXT) \ test-getdtablesize$(EXEEXT) test-getline$(EXEEXT) \ test-getopt-gnu$(EXEEXT) test-getopt-posix$(EXEEXT) \ test-getprogname$(EXEEXT) test-gettimeofday$(EXEEXT) \ test-ignore-value$(EXEEXT) test-inet_pton$(EXEEXT) \ test-intprops$(EXEEXT) test-inttypes$(EXEEXT) \ test-ioctl$(EXEEXT) test-isblank$(EXEEXT) \ test-isnand-nolibm$(EXEEXT) test-isnanf-nolibm$(EXEEXT) \ test-isnanl-nolibm$(EXEEXT) test-iswblank$(EXEEXT) \ test-langinfo$(EXEEXT) test-limits-h$(EXEEXT) \ test-listen$(EXEEXT) test-locale$(EXEEXT) \ test-localeconv$(EXEEXT) test-localename$(EXEEXT) \ test-rwlock1$(EXEEXT) test-lock$(EXEEXT) test-lstat$(EXEEXT) \ test-malloc-gnu$(EXEEXT) test-malloca$(EXEEXT) \ test-math$(EXEEXT) test-mbrtowc1.sh test-mbrtowc2.sh \ test-mbrtowc3.sh test-mbrtowc4.sh test-mbrtowc5.sh \ test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh \ test-mbrtowc-w32-3.sh test-mbrtowc-w32-4.sh \ test-mbrtowc-w32-5.sh test-mbschr.sh test-mbsinit.sh \ test-mbspbrk.sh test-mbsspn.sh test-memchr$(EXEEXT) \ test-nanosleep$(EXEEXT) test-netinet_in$(EXEEXT) \ test-nl_langinfo.sh test-open$(EXEEXT) test-pathmax$(EXEEXT) \ test-perror.sh test-perror2$(EXEEXT) test-pipe$(EXEEXT) \ test-pthread_sigmask1$(EXEEXT) test-pthread_sigmask2$(EXEEXT) \ test-raise$(EXEEXT) test-rawmemchr$(EXEEXT) \ test-regex$(EXEEXT) test-select$(EXEEXT) test-select-in.sh \ test-select-out.sh test-setenv$(EXEEXT) test-setlocale1.sh \ test-setlocale2.sh test-setsockopt$(EXEEXT) \ test-sigaction$(EXEEXT) test-signal-h$(EXEEXT) \ test-signbit$(EXEEXT) test-sigprocmask$(EXEEXT) \ test-sleep$(EXEEXT) test-sockets$(EXEEXT) test-stat$(EXEEXT) \ test-stat-time$(EXEEXT) test-stdalign$(EXEEXT) \ test-stdbool$(EXEEXT) test-stddef$(EXEEXT) \ test-stdint$(EXEEXT) test-stdio$(EXEEXT) test-stdlib$(EXEEXT) \ test-strchrnul$(EXEEXT) test-strerror$(EXEEXT) \ test-strerror_r$(EXEEXT) test-string$(EXEEXT) \ test-strings$(EXEEXT) test-strnlen$(EXEEXT) \ test-strtod$(EXEEXT) test-symlink$(EXEEXT) \ test-sys_ioctl$(EXEEXT) test-sys_select$(EXEEXT) \ test-sys_socket$(EXEEXT) test-sys_stat$(EXEEXT) \ test-sys_time$(EXEEXT) test-sys_types$(EXEEXT) \ test-sys_uio$(EXEEXT) test-sysexits$(EXEEXT) test-init.sh \ test-thread_self$(EXEEXT) test-thread_create$(EXEEXT) \ test-time$(EXEEXT) test-unistd$(EXEEXT) test-uc_width$(EXEEXT) \ uniwidth/test-uc_width2.sh test-unsetenv$(EXEEXT) \ test-usleep$(EXEEXT) test-vasnprintf$(EXEEXT) \ test-verify$(EXEEXT) test-verify.sh test-vsnprintf$(EXEEXT) \ test-wchar$(EXEEXT) test-wcrtomb.sh test-wcrtomb-w32-1.sh \ test-wcrtomb-w32-2.sh test-wcrtomb-w32-3.sh \ test-wcrtomb-w32-4.sh test-wcrtomb-w32-5.sh \ test-wctype-h$(EXEEXT) test-wcwidth$(EXEEXT) XFAIL_TESTS = noinst_PROGRAMS = check_PROGRAMS = test-accept$(EXEEXT) test-alloca-opt$(EXEEXT) \ test-argp$(EXEEXT) test-arpa_inet$(EXEEXT) \ test-binary-io$(EXEEXT) test-bind$(EXEEXT) test-btowc$(EXEEXT) \ test-c-ctype$(EXEEXT) test-c-strcasecmp$(EXEEXT) \ test-c-strncasecmp$(EXEEXT) test-cloexec$(EXEEXT) \ test-close$(EXEEXT) test-connect$(EXEEXT) test-ctype$(EXEEXT) \ test-dup2$(EXEEXT) test-environ$(EXEEXT) test-errno$(EXEEXT) \ test-fcntl-h$(EXEEXT) test-fcntl$(EXEEXT) test-fdopen$(EXEEXT) \ test-fgetc$(EXEEXT) test-float$(EXEEXT) test-fputc$(EXEEXT) \ test-fread$(EXEEXT) test-fstat$(EXEEXT) \ test-ftruncate$(EXEEXT) test-func$(EXEEXT) \ test-fwrite$(EXEEXT) test-getcwd-lgpl$(EXEEXT) \ test-getdelim$(EXEEXT) test-getdtablesize$(EXEEXT) \ test-getline$(EXEEXT) test-getopt-gnu$(EXEEXT) \ test-getopt-posix$(EXEEXT) test-getprogname$(EXEEXT) \ test-gettimeofday$(EXEEXT) test-ignore-value$(EXEEXT) \ test-inet_pton$(EXEEXT) test-intprops$(EXEEXT) \ test-inttypes$(EXEEXT) test-ioctl$(EXEEXT) \ test-isblank$(EXEEXT) test-isnand-nolibm$(EXEEXT) \ test-isnanf-nolibm$(EXEEXT) test-isnanl-nolibm$(EXEEXT) \ test-iswblank$(EXEEXT) test-langinfo$(EXEEXT) \ test-limits-h$(EXEEXT) test-listen$(EXEEXT) \ test-locale$(EXEEXT) test-localeconv$(EXEEXT) \ test-localename$(EXEEXT) test-rwlock1$(EXEEXT) \ test-lock$(EXEEXT) test-lstat$(EXEEXT) \ test-malloc-gnu$(EXEEXT) test-malloca$(EXEEXT) \ test-math$(EXEEXT) test-mbrtowc$(EXEEXT) \ test-mbrtowc-w32$(EXEEXT) test-mbschr$(EXEEXT) \ test-mbsinit$(EXEEXT) test-mbspbrk$(EXEEXT) \ test-mbsspn$(EXEEXT) test-memchr$(EXEEXT) \ test-nanosleep$(EXEEXT) test-netinet_in$(EXEEXT) \ test-nl_langinfo$(EXEEXT) test-open$(EXEEXT) \ test-pathmax$(EXEEXT) test-perror$(EXEEXT) \ 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ALLOCA = @ALLOCA@ ALLOCA_H = @ALLOCA_H@ AMTAR = @AMTAR@ AM_DEFAULT_VERBOSITY = @AM_DEFAULT_VERBOSITY@ APPLE_UNIVERSAL_BUILD = @APPLE_UNIVERSAL_BUILD@ AR = @AR@ ARFLAGS = @ARFLAGS@ AUTOCONF = @AUTOCONF@ AUTOHEADER = @AUTOHEADER@ AUTOMAKE = @AUTOMAKE@ AWK = @AWK@ BITSIZEOF_PTRDIFF_T = @BITSIZEOF_PTRDIFF_T@ BITSIZEOF_SIG_ATOMIC_T = @BITSIZEOF_SIG_ATOMIC_T@ BITSIZEOF_SIZE_T = @BITSIZEOF_SIZE_T@ BITSIZEOF_WCHAR_T = @BITSIZEOF_WCHAR_T@ BITSIZEOF_WINT_T = @BITSIZEOF_WINT_T@ CC = @CC@ CCDEPMODE = @CCDEPMODE@ CFLAGS = @CFLAGS@ CPP = @CPP@ CPPFLAGS = @CPPFLAGS@ CXX = @CXX@ CXXCPP = @CXXCPP@ CXXDEPMODE = @CXXDEPMODE@ CXXFLAGS = @CXXFLAGS@ CYGPATH_W = @CYGPATH_W@ DEFS = @DEFS@ -DEXEEXT=\"@EXEEXT@\" DEPDIR = @DEPDIR@ DLLTOOL = @DLLTOOL@ DSYMUTIL = @DSYMUTIL@ DUMPBIN = @DUMPBIN@ ECHO_C = @ECHO_C@ ECHO_N = @ECHO_N@ ECHO_T = @ECHO_T@ EGREP = @EGREP@ EMULTIHOP_HIDDEN = @EMULTIHOP_HIDDEN@ EMULTIHOP_VALUE = @EMULTIHOP_VALUE@ ENOLINK_HIDDEN = @ENOLINK_HIDDEN@ ENOLINK_VALUE = @ENOLINK_VALUE@ EOVERFLOW_HIDDEN = @EOVERFLOW_HIDDEN@ EOVERFLOW_VALUE = @EOVERFLOW_VALUE@ ERRNO_H = @ERRNO_H@ EXEEXT = @EXEEXT@ FGREP = @FGREP@ FLOAT_H = @FLOAT_H@ GAL_LT_VERSION = @GAL_LT_VERSION@ GETOPT_CDEFS_H = @GETOPT_CDEFS_H@ GETOPT_H = @GETOPT_H@ GLIBC21 = @GLIBC21@ GNULIB_ACCEPT = @GNULIB_ACCEPT@ GNULIB_ACCEPT4 = @GNULIB_ACCEPT4@ GNULIB_ACOSF = @GNULIB_ACOSF@ GNULIB_ACOSL = @GNULIB_ACOSL@ GNULIB_ASINF = @GNULIB_ASINF@ GNULIB_ASINL = @GNULIB_ASINL@ GNULIB_ATAN2F = @GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BIND = @GNULIB_BIND@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINDOWS_STAT_INODES = @WINDOWS_STAT_INODES@ WINDOWS_STAT_TIMESPEC = @WINDOWS_STAT_TIMESPEC@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = @abs_top_srcdir@ ac_ct_AR = @ac_ct_AR@ ac_ct_CC = @ac_ct_CC@ ac_ct_CXX = @ac_ct_CXX@ ac_ct_DUMPBIN = @ac_ct_DUMPBIN@ am__include = @am__include@ am__leading_dot = @am__leading_dot@ am__quote = @am__quote@ am__tar = @am__tar@ am__untar = @am__untar@ ax_pthread_config = @ax_pthread_config@ bindir = @bindir@ build = @build@ build_alias = @build_alias@ build_cpu = @build_cpu@ build_os = @build_os@ build_vendor = @build_vendor@ builddir = @builddir@ datadir = @datadir@ datarootdir = @datarootdir@ docdir = @docdir@ dvidir = @dvidir@ exec_prefix = @exec_prefix@ gl_LIBOBJS = @gl_LIBOBJS@ gl_LTLIBOBJS = @gl_LTLIBOBJS@ gltests_LIBOBJS = @gltests_LIBOBJS@ gltests_LTLIBOBJS = @gltests_LTLIBOBJS@ gltests_WITNESS = @gltests_WITNESS@ has_ghostscript = @has_ghostscript@ has_glibtool = @has_glibtool@ has_help2man = @has_help2man@ has_libtool = @has_libtool@ host = @host@ host_alias = @host_alias@ host_cpu = @host_cpu@ host_os = @host_os@ host_vendor = @host_vendor@ htmldir = @htmldir@ includedir = @includedir@ infodir = @infodir@ install_sh = @install_sh@ libdir = @libdir@ libexecdir = @libexecdir@ lispdir = @lispdir@ localedir = @localedir@ localstatedir = @localstatedir@ mandir = @mandir@ mkdir_p = @mkdir_p@ oldincludedir = @oldincludedir@ pdfdir = @pdfdir@ prefix = @prefix@ program_transform_name = @program_transform_name@ psdir = @psdir@ runstatedir = @runstatedir@ sbindir = @sbindir@ sharedstatedir = @sharedstatedir@ srcdir = @srcdir@ sysconfdir = @sysconfdir@ target_alias = @target_alias@ top_build_prefix = @top_build_prefix@ top_builddir = @top_builddir@ top_srcdir = @top_srcdir@ AUTOMAKE_OPTIONS = 1.9.6 foreign subdir-objects SUBDIRS = . TESTS_ENVIRONMENT = EXEEXT='@EXEEXT@' srcdir='$(srcdir)' \ LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_FR='@LOCALE_FR@' LOCALE_TR_UTF8='@LOCALE_TR_UTF8@' \ LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' LOCALE_ZH_CN='@LOCALE_ZH_CN@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' MAKE='$(MAKE)' \ LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' LOCALE_ZH_CN='@LOCALE_ZH_CN@' noinst_HEADERS = noinst_LIBRARIES = check_LIBRARIES = libtests.a EXTRA_DIST = accept.c w32sock.h test-accept.c signature.h macros.h \ test-alloca-opt.c test-argp.c test-argp-2.sh macros.h \ arpa_inet.in.h test-arpa_inet.c test-binary-io.sh \ test-binary-io.c macros.h bind.c w32sock.h test-bind.c \ signature.h macros.h test-btowc1.sh test-btowc2.sh \ test-btowc.c signature.h macros.h test-c-ctype.c macros.h \ test-c-strcase.sh test-c-strcasecmp.c test-c-strncasecmp.c \ macros.h cloexec.h test-cloexec.c macros.h close.c \ test-close.c signature.h macros.h connect.c w32sock.h \ test-connect.c signature.h macros.h ctype.in.h test-ctype.c \ dup2.c test-dup2.c signature.h macros.h test-environ.c \ test-errno.c fcntl.c fcntl.in.h test-fcntl-h.c test-fcntl.c \ signature.h macros.h fd-hook.h fdopen.c test-fdopen.c \ signature.h macros.h test-fgetc.c signature.h macros.h \ filename.h flexmember.h test-float.c macros.h fpucw.h \ test-fputc.c signature.h macros.h test-fread.c signature.h \ macros.h fstat.c stat-w32.c stat-w32.h test-fstat.c \ signature.h macros.h ftruncate.c test-ftruncate.c \ test-ftruncate.sh signature.h macros.h test-func.c macros.h \ test-fwrite.c signature.h macros.h getcwd-lgpl.c \ test-getcwd-lgpl.c signature.h macros.h test-getdelim.c \ signature.h macros.h getdtablesize.c test-getdtablesize.c \ signature.h macros.h test-getline.c signature.h macros.h \ macros.h signature.h test-getopt-gnu.c test-getopt-main.h \ test-getopt.h test-getopt_long.h macros.h signature.h \ test-getopt-posix.c test-getopt-main.h test-getopt.h \ getpagesize.c test-getprogname.c gettimeofday.c signature.h \ test-gettimeofday.c ignore-value.h test-ignore-value.c \ inet_pton.c test-inet_pton.c signature.h macros.h \ test-intprops.c macros.h test-inttypes.c ioctl.c w32sock.h \ test-ioctl.c signature.h macros.h isblank.c test-isblank.c \ signature.h macros.h float+.h isnan.c isnand-nolibm.h isnand.c \ test-isnand-nolibm.c test-isnand.h minus-zero.h infinity.h \ nan.h macros.h float+.h isnan.c isnanf-nolibm.h isnanf.c \ test-isnanf-nolibm.c test-isnanf.h minus-zero.h infinity.h \ nan.h macros.h float+.h isnan.c isnanl-nolibm.h isnanl.c \ test-isnanl-nolibm.c test-isnanl.h minus-zero.h infinity.h \ nan.h macros.h test-iswblank.c macros.h test-langinfo.c \ test-limits-h.c listen.c w32sock.h test-listen.c signature.h \ macros.h test-locale.c test-localeconv.c signature.h macros.h \ localename.h test-localename.c macros.h localtime-buffer.c \ localtime-buffer.h test-rwlock1.c test-lock.c lstat.c \ test-lstat.h test-lstat.c signature.h macros.h \ test-malloc-gnu.c malloca.h malloca.valgrind test-malloca.c \ test-math.c macros.h test-mbrtowc1.sh test-mbrtowc2.sh \ test-mbrtowc3.sh test-mbrtowc4.sh test-mbrtowc5.sh \ test-mbrtowc.c test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh \ test-mbrtowc-w32-3.sh test-mbrtowc-w32-4.sh \ test-mbrtowc-w32-5.sh test-mbrtowc-w32.c signature.h macros.h \ test-mbschr.sh test-mbschr.c macros.h test-mbsinit.sh \ test-mbsinit.c signature.h macros.h test-mbspbrk.sh \ test-mbspbrk.c macros.h test-mbsspn.sh test-mbsspn.c macros.h \ test-memchr.c zerosize-ptr.h signature.h macros.h nanosleep.c \ test-nanosleep.c signature.h macros.h netinet_in.in.h \ test-netinet_in.c test-nl_langinfo.sh test-nl_langinfo.c \ signature.h macros.h open.c test-open.h test-open.c \ signature.h macros.h pathmax.h test-pathmax.c perror.c \ macros.h signature.h test-perror.c test-perror2.c \ test-perror.sh pipe.c test-pipe.c signature.h macros.h \ pthread_sigmask.c test-pthread_sigmask1.c \ test-pthread_sigmask2.c signature.h macros.h putenv.c raise.c \ test-raise.c signature.h macros.h test-rawmemchr.c \ zerosize-ptr.h signature.h macros.h test-regex.c macros.h \ same-inode.h select.c macros.h signature.h test-select.c \ test-select.h test-select-fd.c test-select-in.sh \ test-select-out.sh test-select-stdin.c setenv.c test-setenv.c \ signature.h macros.h setlocale.c test-setlocale1.sh \ test-setlocale1.c test-setlocale2.sh test-setlocale2.c \ signature.h macros.h setsockopt.c w32sock.h test-setsockopt.c \ signature.h macros.h sig-handler.h sigaction.c \ test-sigaction.c signature.h macros.h signal.in.h \ test-signal-h.c float+.h signbitd.c signbitf.c signbitl.c \ test-signbit.c minus-zero.h infinity.h macros.h sigprocmask.c \ test-sigprocmask.c signature.h macros.h test-sleep.c \ signature.h macros.h _Noreturn.h arg-nonnull.h c++defs.h \ warn-on-use.h socket.c w32sock.h w32sock.h test-sockets.c \ stat-w32.c stat-w32.h stat.c test-stat.h test-stat.c \ signature.h macros.h stat-time.h test-stat-time.c macros.h \ nap.h test-stdalign.c macros.h test-stdbool.c test-stddef.c \ test-stdint.c test-stdio.c test-stdlib.c test-sys_wait.h \ test-strchrnul.c signature.h macros.h test-strerror.c \ signature.h macros.h strerror_r.c test-strerror_r.c \ signature.h macros.h test-string.c test-strings.c \ test-strnlen.c zerosize-ptr.h signature.h macros.h \ test-strtod.c signature.h minus-zero.h macros.h symlink.c \ test-symlink.h test-symlink.c signature.h macros.h \ sys_ioctl.in.h test-sys_ioctl.c sys_select.in.h \ test-sys_select.c signature.h sys_socket.in.h \ test-sys_socket.c sys_stat.in.h test-sys_stat.c sys_time.in.h \ test-sys_time.c test-sys_types.c sys_uio.in.h test-sys_uio.c \ test-sysexits.c init.sh test-init.sh test-thread_self.c \ test-thread_create.c macros.h time.in.h test-time.c \ test-unistd.c uniwidth/test-uc_width.c \ uniwidth/test-uc_width2.c uniwidth/test-uc_width2.sh macros.h \ unsetenv.c test-unsetenv.c signature.h macros.h usleep.c \ test-usleep.c signature.h macros.h test-vasnprintf.c macros.h \ test-verify.c test-verify-try.c test-verify.sh \ test-vsnprintf.c signature.h macros.h test-wchar.c \ test-wcrtomb.sh test-wcrtomb.c test-wcrtomb-w32-1.sh \ test-wcrtomb-w32-2.sh test-wcrtomb-w32-3.sh \ test-wcrtomb-w32-4.sh test-wcrtomb-w32-5.sh test-wcrtomb-w32.c \ signature.h macros.h wctob.c wctomb-impl.h wctomb.c \ test-wctype-h.c macros.h test-wcwidth.c signature.h macros.h \ xalloc-oversized.h BUILT_SOURCES = arpa/inet.h ctype.h fcntl.h $(NETINET_IN_H) signal.h \ sys/ioctl.h sys/select.h sys/socket.h sys/stat.h sys/time.h \ sys/uio.h time.h SUFFIXES = # This test expects compilation of test-verify-try.c to fail, and # each time it fails, the 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GENERATED AUTOMATICALLY! ## Process this file with automake to produce Makefile.in. # Copyright (C) 2002-2017 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. AUTOMAKE_OPTIONS = 1.9.6 foreign subdir-objects SUBDIRS = . TESTS = XFAIL_TESTS = TESTS_ENVIRONMENT = noinst_PROGRAMS = check_PROGRAMS = EXTRA_PROGRAMS = noinst_HEADERS = noinst_LIBRARIES = check_LIBRARIES = libtests.a EXTRA_DIST = BUILT_SOURCES = SUFFIXES = MOSTLYCLEANFILES = core *.stackdump MOSTLYCLEANDIRS = CLEANFILES = DISTCLEANFILES = MAINTAINERCLEANFILES = AM_CPPFLAGS = \ -D@gltests_WITNESS@=1 \ -I. -I$(srcdir) \ -I../.. -I$(srcdir)/../.. \ -I../../bootstrapped/lib -I$(srcdir)/../../bootstrapped/lib LDADD = libtests.a ../../bootstrapped/lib/libgnu.la libtests.a $(LIBTESTS_LIBDEPS) libtests_a_SOURCES = libtests_a_LIBADD = $(gltests_LIBOBJS) libtests_a_DEPENDENCIES = $(gltests_LIBOBJS) EXTRA_libtests_a_SOURCES = AM_LIBTOOLFLAGS = --preserve-dup-deps TESTS_ENVIRONMENT += EXEEXT='@EXEEXT@' srcdir='$(srcdir)' ## begin gnulib module accept EXTRA_DIST += accept.c w32sock.h EXTRA_libtests_a_SOURCES += accept.c ## end gnulib module accept ## begin gnulib module accept-tests TESTS += test-accept check_PROGRAMS += test-accept test_accept_LDADD = $(LDADD) @LIBSOCKET@ EXTRA_DIST += test-accept.c signature.h macros.h ## end gnulib module accept-tests ## begin gnulib module alloca-opt-tests TESTS += test-alloca-opt check_PROGRAMS += test-alloca-opt EXTRA_DIST += test-alloca-opt.c ## end gnulib module alloca-opt-tests ## begin gnulib module argp-tests TESTS += test-argp test-argp-2.sh check_PROGRAMS += test-argp test_argp_LDADD = $(LDADD) @LIBINTL@ EXTRA_DIST += test-argp.c test-argp-2.sh macros.h ## end gnulib module argp-tests ## begin gnulib module arpa_inet BUILT_SOURCES += arpa/inet.h # We need the following in order to create when the system # doesn't have one. arpa/inet.h: arpa_inet.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_at)$(MKDIR_P) arpa $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''HAVE_FEATURES_H''@|$(HAVE_FEATURES_H)|g' \ -e 's|@''NEXT_ARPA_INET_H''@|$(NEXT_ARPA_INET_H)|g' \ -e 's|@''HAVE_ARPA_INET_H''@|$(HAVE_ARPA_INET_H)|g' \ -e 's/@''GNULIB_INET_NTOP''@/$(GNULIB_INET_NTOP)/g' \ -e 's/@''GNULIB_INET_PTON''@/$(GNULIB_INET_PTON)/g' \ -e 's|@''HAVE_DECL_INET_NTOP''@|$(HAVE_DECL_INET_NTOP)|g' \ -e 's|@''HAVE_DECL_INET_PTON''@|$(HAVE_DECL_INET_PTON)|g' \ -e 's|@''REPLACE_INET_NTOP''@|$(REPLACE_INET_NTOP)|g' \ -e 's|@''REPLACE_INET_PTON''@|$(REPLACE_INET_PTON)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/arpa_inet.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += arpa/inet.h arpa/inet.h-t MOSTLYCLEANDIRS += arpa EXTRA_DIST += arpa_inet.in.h ## end gnulib module arpa_inet ## begin gnulib module arpa_inet-tests TESTS += test-arpa_inet check_PROGRAMS += test-arpa_inet EXTRA_DIST += test-arpa_inet.c ## end gnulib module arpa_inet-tests ## begin gnulib module binary-io libtests_a_SOURCES += binary-io.h binary-io.c ## end gnulib module binary-io ## begin gnulib module binary-io-tests TESTS += test-binary-io.sh check_PROGRAMS += test-binary-io EXTRA_DIST += test-binary-io.sh test-binary-io.c macros.h ## end gnulib module binary-io-tests ## begin gnulib module bind EXTRA_DIST += bind.c w32sock.h EXTRA_libtests_a_SOURCES += bind.c ## end gnulib module bind ## begin gnulib module bind-tests TESTS += test-bind check_PROGRAMS += test-bind test_bind_LDADD = $(LDADD) @LIBSOCKET@ $(INET_PTON_LIB) EXTRA_DIST += test-bind.c signature.h macros.h ## end gnulib module bind-tests ## begin gnulib module btowc-tests TESTS += test-btowc1.sh test-btowc2.sh TESTS_ENVIRONMENT += LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-btowc EXTRA_DIST += test-btowc1.sh test-btowc2.sh test-btowc.c signature.h macros.h ## end gnulib module btowc-tests ## begin gnulib module c-ctype-tests TESTS += test-c-ctype check_PROGRAMS += test-c-ctype EXTRA_DIST += test-c-ctype.c macros.h ## end gnulib module c-ctype-tests ## begin gnulib module c-strcase libtests_a_SOURCES += c-strcase.h c-strcasecmp.c c-strncasecmp.c ## end gnulib module c-strcase ## begin gnulib module c-strcase-tests TESTS += test-c-strcase.sh TESTS_ENVIRONMENT += LOCALE_FR='@LOCALE_FR@' LOCALE_TR_UTF8='@LOCALE_TR_UTF8@' check_PROGRAMS += test-c-strcasecmp test-c-strncasecmp EXTRA_DIST += test-c-strcase.sh test-c-strcasecmp.c test-c-strncasecmp.c macros.h ## end gnulib module c-strcase-tests ## begin gnulib module cloexec libtests_a_SOURCES += cloexec.c EXTRA_DIST += cloexec.h ## end gnulib module cloexec ## begin gnulib module cloexec-tests TESTS += test-cloexec check_PROGRAMS += test-cloexec EXTRA_DIST += test-cloexec.c macros.h ## end gnulib module cloexec-tests ## begin gnulib module close EXTRA_DIST += close.c EXTRA_libtests_a_SOURCES += close.c ## end gnulib module close ## begin gnulib module close-tests TESTS += test-close check_PROGRAMS += test-close EXTRA_DIST += test-close.c signature.h macros.h ## end gnulib module close-tests ## begin gnulib module connect EXTRA_DIST += connect.c w32sock.h EXTRA_libtests_a_SOURCES += connect.c ## end gnulib module connect ## begin gnulib module connect-tests TESTS += test-connect check_PROGRAMS += test-connect test_connect_LDADD = $(LDADD) @LIBSOCKET@ $(INET_PTON_LIB) EXTRA_DIST += test-connect.c signature.h macros.h ## end gnulib module connect-tests ## begin gnulib module ctype BUILT_SOURCES += ctype.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. ctype.h: ctype.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_CTYPE_H''@|$(NEXT_CTYPE_H)|g' \ -e 's/@''GNULIB_ISBLANK''@/$(GNULIB_ISBLANK)/g' \ -e 's/@''HAVE_ISBLANK''@/$(HAVE_ISBLANK)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/ctype.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += ctype.h ctype.h-t EXTRA_DIST += ctype.in.h ## end gnulib module ctype ## begin gnulib module ctype-tests TESTS += test-ctype check_PROGRAMS += test-ctype EXTRA_DIST += test-ctype.c ## end gnulib module ctype-tests ## begin gnulib module dup2 EXTRA_DIST += dup2.c EXTRA_libtests_a_SOURCES += dup2.c ## end gnulib module dup2 ## begin gnulib module dup2-tests TESTS += test-dup2 check_PROGRAMS += test-dup2 EXTRA_DIST += test-dup2.c signature.h macros.h ## end gnulib module dup2-tests ## begin gnulib module environ-tests TESTS += test-environ check_PROGRAMS += test-environ EXTRA_DIST += test-environ.c ## end gnulib module environ-tests ## begin gnulib module errno-tests TESTS += test-errno check_PROGRAMS += test-errno EXTRA_DIST += test-errno.c ## end gnulib module errno-tests ## begin gnulib module fcntl EXTRA_DIST += fcntl.c EXTRA_libtests_a_SOURCES += fcntl.c ## end gnulib module fcntl ## begin gnulib module fcntl-h BUILT_SOURCES += fcntl.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. fcntl.h: fcntl.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_FCNTL_H''@|$(NEXT_FCNTL_H)|g' \ -e 's/@''GNULIB_FCNTL''@/$(GNULIB_FCNTL)/g' \ -e 's/@''GNULIB_NONBLOCKING''@/$(GNULIB_NONBLOCKING)/g' \ -e 's/@''GNULIB_OPEN''@/$(GNULIB_OPEN)/g' \ -e 's/@''GNULIB_OPENAT''@/$(GNULIB_OPENAT)/g' \ -e 's|@''HAVE_FCNTL''@|$(HAVE_FCNTL)|g' \ -e 's|@''HAVE_OPENAT''@|$(HAVE_OPENAT)|g' \ -e 's|@''REPLACE_FCNTL''@|$(REPLACE_FCNTL)|g' \ -e 's|@''REPLACE_OPEN''@|$(REPLACE_OPEN)|g' \ -e 's|@''REPLACE_OPENAT''@|$(REPLACE_OPENAT)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/fcntl.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += fcntl.h fcntl.h-t EXTRA_DIST += fcntl.in.h ## end gnulib module fcntl-h ## begin gnulib module fcntl-h-tests TESTS += test-fcntl-h check_PROGRAMS += test-fcntl-h EXTRA_DIST += test-fcntl-h.c ## end gnulib module fcntl-h-tests ## begin gnulib module fcntl-tests TESTS += test-fcntl check_PROGRAMS += test-fcntl EXTRA_DIST += test-fcntl.c signature.h macros.h ## end gnulib module fcntl-tests ## begin gnulib module fd-hook libtests_a_SOURCES += fd-hook.c EXTRA_DIST += fd-hook.h ## end gnulib module fd-hook ## begin gnulib module fdopen EXTRA_DIST += fdopen.c EXTRA_libtests_a_SOURCES += fdopen.c ## end gnulib module fdopen ## begin gnulib module fdopen-tests TESTS += test-fdopen check_PROGRAMS += test-fdopen EXTRA_DIST += test-fdopen.c signature.h macros.h ## end gnulib module fdopen-tests ## begin gnulib module fgetc-tests TESTS += test-fgetc check_PROGRAMS += test-fgetc EXTRA_DIST += test-fgetc.c signature.h macros.h ## end gnulib module fgetc-tests ## begin gnulib module filename EXTRA_DIST += filename.h ## end gnulib module filename ## begin gnulib module flexmember EXTRA_DIST += flexmember.h ## end gnulib module flexmember ## begin gnulib module float-tests TESTS += test-float check_PROGRAMS += test-float EXTRA_DIST += test-float.c macros.h ## end gnulib module float-tests ## begin gnulib module fpucw EXTRA_DIST += fpucw.h ## end gnulib module fpucw ## begin gnulib module fputc-tests TESTS += test-fputc check_PROGRAMS += test-fputc EXTRA_DIST += test-fputc.c signature.h macros.h ## end gnulib module fputc-tests ## begin gnulib module fread-tests TESTS += test-fread check_PROGRAMS += test-fread EXTRA_DIST += test-fread.c signature.h macros.h ## end gnulib module fread-tests ## begin gnulib module fstat EXTRA_DIST += fstat.c stat-w32.c stat-w32.h EXTRA_libtests_a_SOURCES += fstat.c stat-w32.c ## end gnulib module fstat ## begin gnulib module fstat-tests TESTS += test-fstat check_PROGRAMS += test-fstat EXTRA_DIST += test-fstat.c signature.h macros.h ## end gnulib module fstat-tests ## begin gnulib module ftruncate EXTRA_DIST += ftruncate.c EXTRA_libtests_a_SOURCES += ftruncate.c ## end gnulib module ftruncate ## begin gnulib module ftruncate-tests TESTS += test-ftruncate.sh check_PROGRAMS += test-ftruncate EXTRA_DIST += test-ftruncate.c test-ftruncate.sh signature.h macros.h ## end gnulib module ftruncate-tests ## begin gnulib module func-tests TESTS += test-func check_PROGRAMS += test-func EXTRA_DIST += test-func.c macros.h ## end gnulib module func-tests ## begin gnulib module fwrite-tests TESTS += test-fwrite check_PROGRAMS += test-fwrite EXTRA_DIST += test-fwrite.c signature.h macros.h ## end gnulib module fwrite-tests ## begin gnulib module getcwd-lgpl EXTRA_DIST += getcwd-lgpl.c EXTRA_libtests_a_SOURCES += getcwd-lgpl.c ## end gnulib module getcwd-lgpl ## begin gnulib module getcwd-lgpl-tests TESTS += test-getcwd-lgpl check_PROGRAMS += test-getcwd-lgpl test_getcwd_lgpl_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += test-getcwd-lgpl.c signature.h macros.h ## end gnulib module getcwd-lgpl-tests ## begin gnulib module getdelim-tests TESTS += test-getdelim check_PROGRAMS += test-getdelim MOSTLYCLEANFILES += test-getdelim.txt EXTRA_DIST += test-getdelim.c signature.h macros.h ## end gnulib module getdelim-tests ## begin gnulib module getdtablesize EXTRA_DIST += getdtablesize.c EXTRA_libtests_a_SOURCES += getdtablesize.c ## end gnulib module getdtablesize ## begin gnulib module getdtablesize-tests TESTS += test-getdtablesize check_PROGRAMS += test-getdtablesize EXTRA_DIST += test-getdtablesize.c signature.h macros.h ## end gnulib module getdtablesize-tests ## begin gnulib module getline-tests TESTS += test-getline check_PROGRAMS += test-getline MOSTLYCLEANFILES += test-getline.txt EXTRA_DIST += test-getline.c signature.h macros.h ## end gnulib module getline-tests ## begin gnulib module getopt-gnu-tests TESTS += test-getopt-gnu check_PROGRAMS += test-getopt-gnu test_getopt_gnu_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += macros.h signature.h test-getopt-gnu.c test-getopt-main.h test-getopt.h test-getopt_long.h ## end gnulib module getopt-gnu-tests ## begin gnulib module getopt-posix-tests TESTS += test-getopt-posix check_PROGRAMS += test-getopt-posix test_getopt_posix_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += macros.h signature.h test-getopt-posix.c test-getopt-main.h test-getopt.h ## end gnulib module getopt-posix-tests ## begin gnulib module getpagesize EXTRA_DIST += getpagesize.c EXTRA_libtests_a_SOURCES += getpagesize.c ## end gnulib module getpagesize ## begin gnulib module getprogname-tests DEFS += -DEXEEXT=\"@EXEEXT@\" TESTS += test-getprogname check_PROGRAMS += test-getprogname test_getprogname_LDADD = $(LDADD) EXTRA_DIST += test-getprogname.c ## end gnulib module getprogname-tests ## begin gnulib module gettimeofday EXTRA_DIST += gettimeofday.c EXTRA_libtests_a_SOURCES += gettimeofday.c ## end gnulib module gettimeofday ## begin gnulib module gettimeofday-tests TESTS += test-gettimeofday check_PROGRAMS += test-gettimeofday EXTRA_DIST += signature.h test-gettimeofday.c ## end gnulib module gettimeofday-tests ## begin gnulib module ignore-value EXTRA_DIST += ignore-value.h ## end gnulib module ignore-value ## begin gnulib module ignore-value-tests TESTS += test-ignore-value check_PROGRAMS += test-ignore-value EXTRA_DIST += test-ignore-value.c ## end gnulib module ignore-value-tests ## begin gnulib module inet_pton EXTRA_DIST += inet_pton.c EXTRA_libtests_a_SOURCES += inet_pton.c ## end gnulib module inet_pton ## begin gnulib module inet_pton-tests TESTS += test-inet_pton check_PROGRAMS += test-inet_pton test_inet_pton_LDADD = $(LDADD) @INET_PTON_LIB@ EXTRA_DIST += test-inet_pton.c signature.h macros.h ## end gnulib module inet_pton-tests ## begin gnulib module intprops-tests TESTS += test-intprops check_PROGRAMS += test-intprops EXTRA_DIST += test-intprops.c macros.h ## end gnulib module intprops-tests ## begin gnulib module inttypes-tests TESTS += test-inttypes check_PROGRAMS += test-inttypes EXTRA_DIST += test-inttypes.c ## end gnulib module inttypes-tests ## begin gnulib module ioctl EXTRA_DIST += ioctl.c w32sock.h EXTRA_libtests_a_SOURCES += ioctl.c ## end gnulib module ioctl ## begin gnulib module ioctl-tests TESTS += test-ioctl check_PROGRAMS += test-ioctl EXTRA_DIST += test-ioctl.c signature.h macros.h ## end gnulib module ioctl-tests ## begin gnulib module isblank EXTRA_DIST += isblank.c EXTRA_libtests_a_SOURCES += isblank.c ## end gnulib module isblank ## begin gnulib module isblank-tests TESTS += test-isblank check_PROGRAMS += test-isblank EXTRA_DIST += test-isblank.c signature.h macros.h ## end gnulib module isblank-tests ## begin gnulib module isnand-nolibm EXTRA_DIST += float+.h isnan.c isnand-nolibm.h isnand.c EXTRA_libtests_a_SOURCES += isnan.c isnand.c ## end gnulib module isnand-nolibm ## begin gnulib module isnand-nolibm-tests TESTS += test-isnand-nolibm check_PROGRAMS += test-isnand-nolibm EXTRA_DIST += test-isnand-nolibm.c test-isnand.h minus-zero.h infinity.h nan.h macros.h ## end gnulib module isnand-nolibm-tests ## begin gnulib module isnanf-nolibm EXTRA_DIST += float+.h isnan.c isnanf-nolibm.h isnanf.c EXTRA_libtests_a_SOURCES += isnan.c isnanf.c ## end gnulib module isnanf-nolibm ## begin gnulib module isnanf-nolibm-tests TESTS += test-isnanf-nolibm check_PROGRAMS += test-isnanf-nolibm EXTRA_DIST += test-isnanf-nolibm.c test-isnanf.h minus-zero.h infinity.h nan.h macros.h ## end gnulib module isnanf-nolibm-tests ## begin gnulib module isnanl-nolibm EXTRA_DIST += float+.h isnan.c isnanl-nolibm.h isnanl.c EXTRA_libtests_a_SOURCES += isnan.c isnanl.c ## end gnulib module isnanl-nolibm ## begin gnulib module isnanl-nolibm-tests TESTS += test-isnanl-nolibm check_PROGRAMS += test-isnanl-nolibm EXTRA_DIST += test-isnanl-nolibm.c test-isnanl.h minus-zero.h infinity.h nan.h macros.h ## end gnulib module isnanl-nolibm-tests ## begin gnulib module iswblank-tests TESTS += test-iswblank check_PROGRAMS += test-iswblank EXTRA_DIST += test-iswblank.c macros.h ## end gnulib module iswblank-tests ## begin gnulib module langinfo-tests TESTS += test-langinfo check_PROGRAMS += test-langinfo EXTRA_DIST += test-langinfo.c ## end gnulib module langinfo-tests ## begin gnulib module limits-h-tests TESTS += test-limits-h check_PROGRAMS += test-limits-h EXTRA_DIST += test-limits-h.c ## end gnulib module limits-h-tests ## begin gnulib module listen EXTRA_DIST += listen.c w32sock.h EXTRA_libtests_a_SOURCES += listen.c ## end gnulib module listen ## begin gnulib module listen-tests TESTS += test-listen check_PROGRAMS += test-listen test_listen_LDADD = $(LDADD) @LIBSOCKET@ EXTRA_DIST += test-listen.c signature.h macros.h ## end gnulib module listen-tests ## begin gnulib module locale-tests TESTS += test-locale check_PROGRAMS += test-locale EXTRA_DIST += test-locale.c ## end gnulib module locale-tests ## begin gnulib module localeconv-tests TESTS += test-localeconv check_PROGRAMS += test-localeconv EXTRA_DIST += test-localeconv.c signature.h macros.h ## end gnulib module localeconv-tests ## begin gnulib module localename libtests_a_SOURCES += localename.c EXTRA_DIST += localename.h ## end gnulib module localename ## begin gnulib module localename-tests TESTS += test-localename check_PROGRAMS += test-localename test_localename_LDADD = $(LDADD) @INTL_MACOSX_LIBS@ $(LIBTHREAD) EXTRA_DIST += test-localename.c macros.h ## end gnulib module localename-tests ## begin gnulib module localtime-buffer EXTRA_DIST += localtime-buffer.c localtime-buffer.h EXTRA_libtests_a_SOURCES += localtime-buffer.c ## end gnulib module localtime-buffer ## begin gnulib module lock-tests TESTS += test-rwlock1 test-lock check_PROGRAMS += test-rwlock1 test-lock test_rwlock1_LDADD = $(LDADD) @LIBMULTITHREAD@ @YIELD_LIB@ test_lock_LDADD = $(LDADD) @LIBMULTITHREAD@ @YIELD_LIB@ EXTRA_DIST += test-rwlock1.c test-lock.c ## end gnulib module lock-tests ## begin gnulib module lstat EXTRA_DIST += lstat.c EXTRA_libtests_a_SOURCES += lstat.c ## end gnulib module lstat ## begin gnulib module lstat-tests TESTS += test-lstat check_PROGRAMS += test-lstat EXTRA_DIST += test-lstat.h test-lstat.c signature.h macros.h ## end gnulib module lstat-tests ## begin gnulib module malloc-gnu-tests TESTS += test-malloc-gnu check_PROGRAMS += test-malloc-gnu EXTRA_DIST += test-malloc-gnu.c ## end gnulib module malloc-gnu-tests ## begin gnulib module malloca libtests_a_SOURCES += malloca.c EXTRA_DIST += malloca.h malloca.valgrind ## end gnulib module malloca ## begin gnulib module malloca-tests TESTS += test-malloca check_PROGRAMS += test-malloca EXTRA_DIST += test-malloca.c ## end gnulib module malloca-tests ## begin gnulib module math-tests TESTS += test-math check_PROGRAMS += test-math EXTRA_DIST += test-math.c macros.h ## end gnulib module math-tests ## begin gnulib module mbrtowc-tests TESTS += \ test-mbrtowc1.sh test-mbrtowc2.sh test-mbrtowc3.sh test-mbrtowc4.sh \ test-mbrtowc5.sh \ test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh test-mbrtowc-w32-3.sh \ test-mbrtowc-w32-4.sh test-mbrtowc-w32-5.sh TESTS_ENVIRONMENT += \ LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-mbrtowc test-mbrtowc-w32 EXTRA_DIST += test-mbrtowc1.sh test-mbrtowc2.sh test-mbrtowc3.sh test-mbrtowc4.sh test-mbrtowc5.sh test-mbrtowc.c test-mbrtowc-w32-1.sh test-mbrtowc-w32-2.sh test-mbrtowc-w32-3.sh test-mbrtowc-w32-4.sh test-mbrtowc-w32-5.sh test-mbrtowc-w32.c signature.h macros.h ## end gnulib module mbrtowc-tests ## begin gnulib module mbschr-tests TESTS += test-mbschr.sh TESTS_ENVIRONMENT += LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-mbschr EXTRA_DIST += test-mbschr.sh test-mbschr.c macros.h ## end gnulib module mbschr-tests ## begin gnulib module mbsinit-tests TESTS += test-mbsinit.sh TESTS_ENVIRONMENT += LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-mbsinit EXTRA_DIST += test-mbsinit.sh test-mbsinit.c signature.h macros.h ## end gnulib module mbsinit-tests ## begin gnulib module mbspbrk-tests TESTS += test-mbspbrk.sh TESTS_ENVIRONMENT += LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-mbspbrk EXTRA_DIST += test-mbspbrk.sh test-mbspbrk.c macros.h ## end gnulib module mbspbrk-tests ## begin gnulib module mbsspn-tests TESTS += test-mbsspn.sh TESTS_ENVIRONMENT += LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-mbsspn EXTRA_DIST += test-mbsspn.sh test-mbsspn.c macros.h ## end gnulib module mbsspn-tests ## begin gnulib module memchr-tests TESTS += test-memchr check_PROGRAMS += test-memchr EXTRA_DIST += test-memchr.c zerosize-ptr.h signature.h macros.h ## end gnulib module memchr-tests ## begin gnulib module nanosleep EXTRA_DIST += nanosleep.c EXTRA_libtests_a_SOURCES += nanosleep.c ## end gnulib module nanosleep ## begin gnulib module nanosleep-tests TESTS += test-nanosleep check_PROGRAMS += test-nanosleep test_nanosleep_LDADD = $(LDADD) $(LIB_NANOSLEEP) EXTRA_DIST += test-nanosleep.c signature.h macros.h ## end gnulib module nanosleep-tests ## begin gnulib module netinet_in BUILT_SOURCES += $(NETINET_IN_H) # We need the following in order to create when the system # doesn't have one. if GL_GENERATE_NETINET_IN_H netinet/in.h: netinet_in.in.h $(top_builddir)/config.status $(AM_V_at)$(MKDIR_P) netinet $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_NETINET_IN_H''@|$(NEXT_NETINET_IN_H)|g' \ -e 's|@''HAVE_NETINET_IN_H''@|$(HAVE_NETINET_IN_H)|g' \ < $(srcdir)/netinet_in.in.h; \ } > $@-t && \ mv $@-t $@ else netinet/in.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += netinet/in.h netinet/in.h-t MOSTLYCLEANDIRS += netinet EXTRA_DIST += netinet_in.in.h ## end gnulib module netinet_in ## begin gnulib module netinet_in-tests TESTS += test-netinet_in check_PROGRAMS += test-netinet_in EXTRA_DIST += test-netinet_in.c ## end gnulib module netinet_in-tests ## begin gnulib module nl_langinfo-tests TESTS += test-nl_langinfo.sh TESTS_ENVIRONMENT += LOCALE_FR='@LOCALE_FR@' LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' check_PROGRAMS += test-nl_langinfo EXTRA_DIST += test-nl_langinfo.sh test-nl_langinfo.c signature.h macros.h ## end gnulib module nl_langinfo-tests ## begin gnulib module open EXTRA_DIST += open.c EXTRA_libtests_a_SOURCES += open.c ## end gnulib module open ## begin gnulib module open-tests TESTS += test-open check_PROGRAMS += test-open EXTRA_DIST += test-open.h test-open.c signature.h macros.h ## end gnulib module open-tests ## begin gnulib module pathmax EXTRA_DIST += pathmax.h ## end gnulib module pathmax ## begin gnulib module pathmax-tests TESTS += test-pathmax check_PROGRAMS += test-pathmax EXTRA_DIST += test-pathmax.c ## end gnulib module pathmax-tests ## begin gnulib module perror EXTRA_DIST += perror.c EXTRA_libtests_a_SOURCES += perror.c ## end gnulib module perror ## begin gnulib module perror-tests TESTS += test-perror.sh test-perror2 check_PROGRAMS += test-perror test-perror2 EXTRA_DIST += macros.h signature.h test-perror.c test-perror2.c test-perror.sh ## end gnulib module perror-tests ## begin gnulib module pipe-posix EXTRA_DIST += pipe.c EXTRA_libtests_a_SOURCES += pipe.c ## end gnulib module pipe-posix ## begin gnulib module pipe-posix-tests TESTS += test-pipe check_PROGRAMS += test-pipe EXTRA_DIST += test-pipe.c signature.h macros.h ## end gnulib module pipe-posix-tests ## begin gnulib module pthread_sigmask EXTRA_DIST += pthread_sigmask.c EXTRA_libtests_a_SOURCES += pthread_sigmask.c ## end gnulib module pthread_sigmask ## begin gnulib module pthread_sigmask-tests TESTS += test-pthread_sigmask1 test-pthread_sigmask2 check_PROGRAMS += test-pthread_sigmask1 test-pthread_sigmask2 test_pthread_sigmask1_LDADD = $(LDADD) @LIB_PTHREAD_SIGMASK@ test_pthread_sigmask2_LDADD = $(LDADD) @LIB_PTHREAD_SIGMASK@ @LIBMULTITHREAD@ EXTRA_DIST += test-pthread_sigmask1.c test-pthread_sigmask2.c signature.h macros.h ## end gnulib module pthread_sigmask-tests ## begin gnulib module putenv EXTRA_DIST += putenv.c EXTRA_libtests_a_SOURCES += putenv.c ## end gnulib module putenv ## begin gnulib module raise EXTRA_DIST += raise.c EXTRA_libtests_a_SOURCES += raise.c ## end gnulib module raise ## begin gnulib module raise-tests TESTS += test-raise check_PROGRAMS += test-raise EXTRA_DIST += test-raise.c signature.h macros.h ## end gnulib module raise-tests ## begin gnulib module rawmemchr-tests TESTS += test-rawmemchr check_PROGRAMS += test-rawmemchr EXTRA_DIST += test-rawmemchr.c zerosize-ptr.h signature.h macros.h ## end gnulib module rawmemchr-tests ## begin gnulib module regex-tests TESTS += test-regex check_PROGRAMS += test-regex test_regex_LDADD = $(LDADD) @LIBINTL@ $(LIBTHREAD) $(LIB_PTHREAD) EXTRA_DIST += test-regex.c macros.h ## end gnulib module regex-tests ## begin gnulib module same-inode EXTRA_DIST += same-inode.h ## end gnulib module same-inode ## begin gnulib module select EXTRA_DIST += select.c EXTRA_libtests_a_SOURCES += select.c ## end gnulib module select ## begin gnulib module select-tests TESTS += test-select test-select-in.sh test-select-out.sh # test-select-stdin has to be run by hand. check_PROGRAMS += test-select test-select-fd test-select-stdin test_select_LDADD = $(LDADD) @LIB_SELECT@ @LIBSOCKET@ $(INET_PTON_LIB) test_select_fd_LDADD = $(LDADD) @LIB_SELECT@ test_select_stdin_LDADD = $(LDADD) @LIB_SELECT@ EXTRA_DIST += macros.h signature.h test-select.c test-select.h test-select-fd.c test-select-in.sh test-select-out.sh test-select-stdin.c ## end gnulib module select-tests ## begin gnulib module setenv EXTRA_DIST += setenv.c EXTRA_libtests_a_SOURCES += setenv.c ## end gnulib module setenv ## begin gnulib module setenv-tests TESTS += test-setenv check_PROGRAMS += test-setenv EXTRA_DIST += test-setenv.c signature.h macros.h ## end gnulib module setenv-tests ## begin gnulib module setlocale EXTRA_DIST += setlocale.c EXTRA_libtests_a_SOURCES += setlocale.c ## end gnulib module setlocale ## begin gnulib module setlocale-tests TESTS += test-setlocale1.sh test-setlocale2.sh TESTS_ENVIRONMENT += \ LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-setlocale1 test-setlocale2 EXTRA_DIST += test-setlocale1.sh test-setlocale1.c test-setlocale2.sh test-setlocale2.c signature.h macros.h ## end gnulib module setlocale-tests ## begin gnulib module setsockopt EXTRA_DIST += setsockopt.c w32sock.h EXTRA_libtests_a_SOURCES += setsockopt.c ## end gnulib module setsockopt ## begin gnulib module setsockopt-tests TESTS += test-setsockopt check_PROGRAMS += test-setsockopt test_setsockopt_LDADD = $(LDADD) @LIBSOCKET@ EXTRA_DIST += test-setsockopt.c signature.h macros.h ## end gnulib module setsockopt-tests ## begin gnulib module sigaction libtests_a_SOURCES += sig-handler.c EXTRA_DIST += sig-handler.h sigaction.c EXTRA_libtests_a_SOURCES += sigaction.c ## end gnulib module sigaction ## begin gnulib module sigaction-tests TESTS += test-sigaction check_PROGRAMS += test-sigaction EXTRA_DIST += test-sigaction.c signature.h macros.h ## end gnulib module sigaction-tests ## begin gnulib module signal-h BUILT_SOURCES += signal.h # We need the following in order to create when the system # doesn't have a complete one. signal.h: signal.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SIGNAL_H''@|$(NEXT_SIGNAL_H)|g' \ -e 's|@''GNULIB_PTHREAD_SIGMASK''@|$(GNULIB_PTHREAD_SIGMASK)|g' \ -e 's|@''GNULIB_RAISE''@|$(GNULIB_RAISE)|g' \ -e 's/@''GNULIB_SIGNAL_H_SIGPIPE''@/$(GNULIB_SIGNAL_H_SIGPIPE)/g' \ -e 's/@''GNULIB_SIGPROCMASK''@/$(GNULIB_SIGPROCMASK)/g' \ -e 's/@''GNULIB_SIGACTION''@/$(GNULIB_SIGACTION)/g' \ -e 's|@''HAVE_POSIX_SIGNALBLOCKING''@|$(HAVE_POSIX_SIGNALBLOCKING)|g' \ -e 's|@''HAVE_PTHREAD_SIGMASK''@|$(HAVE_PTHREAD_SIGMASK)|g' \ -e 's|@''HAVE_RAISE''@|$(HAVE_RAISE)|g' \ -e 's|@''HAVE_SIGSET_T''@|$(HAVE_SIGSET_T)|g' \ -e 's|@''HAVE_SIGINFO_T''@|$(HAVE_SIGINFO_T)|g' \ -e 's|@''HAVE_SIGACTION''@|$(HAVE_SIGACTION)|g' \ -e 's|@''HAVE_STRUCT_SIGACTION_SA_SIGACTION''@|$(HAVE_STRUCT_SIGACTION_SA_SIGACTION)|g' \ -e 's|@''HAVE_TYPE_VOLATILE_SIG_ATOMIC_T''@|$(HAVE_TYPE_VOLATILE_SIG_ATOMIC_T)|g' \ -e 's|@''HAVE_SIGHANDLER_T''@|$(HAVE_SIGHANDLER_T)|g' \ -e 's|@''REPLACE_PTHREAD_SIGMASK''@|$(REPLACE_PTHREAD_SIGMASK)|g' \ -e 's|@''REPLACE_RAISE''@|$(REPLACE_RAISE)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/signal.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += signal.h signal.h-t EXTRA_DIST += signal.in.h ## end gnulib module signal-h ## begin gnulib module signal-h-tests TESTS += test-signal-h check_PROGRAMS += test-signal-h EXTRA_DIST += test-signal-h.c ## end gnulib module signal-h-tests ## begin gnulib module signbit EXTRA_DIST += float+.h signbitd.c signbitf.c signbitl.c EXTRA_libtests_a_SOURCES += signbitd.c signbitf.c signbitl.c ## end gnulib module signbit ## begin gnulib module signbit-tests TESTS += test-signbit check_PROGRAMS += test-signbit EXTRA_DIST += test-signbit.c minus-zero.h infinity.h macros.h ## end gnulib module signbit-tests ## begin gnulib module sigprocmask EXTRA_DIST += sigprocmask.c EXTRA_libtests_a_SOURCES += sigprocmask.c ## end gnulib module sigprocmask ## begin gnulib module sigprocmask-tests TESTS += test-sigprocmask check_PROGRAMS += test-sigprocmask EXTRA_DIST += test-sigprocmask.c signature.h macros.h ## end gnulib module sigprocmask-tests ## begin gnulib module sleep-tests TESTS += test-sleep check_PROGRAMS += test-sleep EXTRA_DIST += test-sleep.c signature.h macros.h ## end gnulib module sleep-tests ## begin gnulib module snippet/_Noreturn # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. _NORETURN_H=$(srcdir)/_Noreturn.h EXTRA_DIST += _Noreturn.h ## end gnulib module snippet/_Noreturn ## begin gnulib module snippet/arg-nonnull # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. ARG_NONNULL_H=$(srcdir)/arg-nonnull.h EXTRA_DIST += arg-nonnull.h ## end gnulib module snippet/arg-nonnull ## begin gnulib module snippet/c++defs # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. CXXDEFS_H=$(srcdir)/c++defs.h EXTRA_DIST += c++defs.h ## end gnulib module snippet/c++defs ## begin gnulib module snippet/warn-on-use # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. WARN_ON_USE_H=$(srcdir)/warn-on-use.h EXTRA_DIST += warn-on-use.h ## end gnulib module snippet/warn-on-use ## begin gnulib module socket EXTRA_DIST += socket.c w32sock.h EXTRA_libtests_a_SOURCES += socket.c ## end gnulib module socket ## begin gnulib module sockets libtests_a_SOURCES += sockets.h sockets.c EXTRA_DIST += w32sock.h ## end gnulib module sockets ## begin gnulib module sockets-tests TESTS += test-sockets check_PROGRAMS += test-sockets test_sockets_LDADD = $(LDADD) @LIBSOCKET@ EXTRA_DIST += test-sockets.c ## end gnulib module sockets-tests ## begin gnulib module stat EXTRA_DIST += stat-w32.c stat-w32.h stat.c EXTRA_libtests_a_SOURCES += stat-w32.c stat.c ## end gnulib module stat ## begin gnulib module stat-tests TESTS += test-stat check_PROGRAMS += test-stat test_stat_LDADD = $(LDADD) $(LIBINTL) EXTRA_DIST += test-stat.h test-stat.c signature.h macros.h ## end gnulib module stat-tests ## begin gnulib module stat-time libtests_a_SOURCES += stat-time.c EXTRA_DIST += stat-time.h ## end gnulib module stat-time ## begin gnulib module stat-time-tests TESTS += test-stat-time check_PROGRAMS += test-stat-time test_stat_time_LDADD = $(LDADD) $(LIB_NANOSLEEP) EXTRA_DIST += test-stat-time.c macros.h nap.h ## end gnulib module stat-time-tests ## begin gnulib module stdalign-tests TESTS += test-stdalign check_PROGRAMS += test-stdalign EXTRA_DIST += test-stdalign.c macros.h ## end gnulib module stdalign-tests ## begin gnulib module stdbool-tests TESTS += test-stdbool check_PROGRAMS += test-stdbool EXTRA_DIST += test-stdbool.c ## end gnulib module stdbool-tests ## begin gnulib module stddef-tests TESTS += test-stddef check_PROGRAMS += test-stddef EXTRA_DIST += test-stddef.c ## end gnulib module stddef-tests ## begin gnulib module stdint-tests TESTS += test-stdint check_PROGRAMS += test-stdint EXTRA_DIST += test-stdint.c ## end gnulib module stdint-tests ## begin gnulib module stdio-tests TESTS += test-stdio check_PROGRAMS += test-stdio EXTRA_DIST += test-stdio.c ## end gnulib module stdio-tests ## begin gnulib module stdlib-tests TESTS += test-stdlib check_PROGRAMS += test-stdlib EXTRA_DIST += test-stdlib.c test-sys_wait.h ## end gnulib module stdlib-tests ## begin gnulib module strchrnul-tests TESTS += test-strchrnul check_PROGRAMS += test-strchrnul EXTRA_DIST += test-strchrnul.c signature.h macros.h ## end gnulib module strchrnul-tests ## begin gnulib module strerror-tests TESTS += test-strerror check_PROGRAMS += test-strerror EXTRA_DIST += test-strerror.c signature.h macros.h ## end gnulib module strerror-tests ## begin gnulib module strerror_r-posix EXTRA_DIST += strerror_r.c EXTRA_libtests_a_SOURCES += strerror_r.c ## end gnulib module strerror_r-posix ## begin gnulib module strerror_r-posix-tests TESTS += test-strerror_r check_PROGRAMS += test-strerror_r EXTRA_DIST += test-strerror_r.c signature.h macros.h ## end gnulib module strerror_r-posix-tests ## begin gnulib module string-tests TESTS += test-string check_PROGRAMS += test-string EXTRA_DIST += test-string.c ## end gnulib module string-tests ## begin gnulib module strings-tests TESTS += test-strings check_PROGRAMS += test-strings EXTRA_DIST += test-strings.c ## end gnulib module strings-tests ## begin gnulib module strnlen-tests TESTS += test-strnlen check_PROGRAMS += test-strnlen EXTRA_DIST += test-strnlen.c zerosize-ptr.h signature.h macros.h ## end gnulib module strnlen-tests ## begin gnulib module strtod-tests TESTS += test-strtod check_PROGRAMS += test-strtod EXTRA_DIST += test-strtod.c signature.h minus-zero.h macros.h ## end gnulib module strtod-tests ## begin gnulib module symlink EXTRA_DIST += symlink.c EXTRA_libtests_a_SOURCES += symlink.c ## end gnulib module symlink ## begin gnulib module symlink-tests TESTS += test-symlink check_PROGRAMS += test-symlink EXTRA_DIST += test-symlink.h test-symlink.c signature.h macros.h ## end gnulib module symlink-tests ## begin gnulib module sys_ioctl BUILT_SOURCES += sys/ioctl.h # We need the following in order to create when the system # does not have a complete one. sys/ioctl.h: sys_ioctl.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_SYS_IOCTL_H''@|$(HAVE_SYS_IOCTL_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_IOCTL_H''@|$(NEXT_SYS_IOCTL_H)|g' \ -e 's/@''GNULIB_IOCTL''@/$(GNULIB_IOCTL)/g' \ -e 's|@''SYS_IOCTL_H_HAVE_WINSOCK2_H''@|$(SYS_IOCTL_H_HAVE_WINSOCK2_H)|g' \ -e 's|@''SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS''@|$(SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS)|g' \ -e 's|@''REPLACE_IOCTL''@|$(REPLACE_IOCTL)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_ioctl.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/ioctl.h sys/ioctl.h-t MOSTLYCLEANDIRS += sys EXTRA_DIST += sys_ioctl.in.h ## end gnulib module sys_ioctl ## begin gnulib module sys_ioctl-tests TESTS += test-sys_ioctl check_PROGRAMS += test-sys_ioctl EXTRA_DIST += test-sys_ioctl.c ## end gnulib module sys_ioctl-tests ## begin gnulib module sys_select BUILT_SOURCES += sys/select.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/select.h: sys_select.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_SELECT_H''@|$(NEXT_SYS_SELECT_H)|g' \ -e 's|@''HAVE_SYS_SELECT_H''@|$(HAVE_SYS_SELECT_H)|g' \ -e 's/@''GNULIB_PSELECT''@/$(GNULIB_PSELECT)/g' \ -e 's/@''GNULIB_SELECT''@/$(GNULIB_SELECT)/g' \ -e 's|@''HAVE_WINSOCK2_H''@|$(HAVE_WINSOCK2_H)|g' \ -e 's|@''HAVE_PSELECT''@|$(HAVE_PSELECT)|g' \ -e 's|@''REPLACE_PSELECT''@|$(REPLACE_PSELECT)|g' \ -e 's|@''REPLACE_SELECT''@|$(REPLACE_SELECT)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_select.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/select.h sys/select.h-t MOSTLYCLEANDIRS += sys EXTRA_DIST += sys_select.in.h ## end gnulib module sys_select ## begin gnulib module sys_select-tests TESTS += test-sys_select check_PROGRAMS += test-sys_select EXTRA_DIST += test-sys_select.c signature.h ## end gnulib module sys_select-tests ## begin gnulib module sys_socket BUILT_SOURCES += sys/socket.h libtests_a_SOURCES += sys_socket.c # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/socket.h: sys_socket.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_SOCKET_H''@|$(NEXT_SYS_SOCKET_H)|g' \ -e 's|@''HAVE_SYS_SOCKET_H''@|$(HAVE_SYS_SOCKET_H)|g' \ -e 's/@''GNULIB_CLOSE''@/$(GNULIB_CLOSE)/g' \ -e 's/@''GNULIB_SOCKET''@/$(GNULIB_SOCKET)/g' \ -e 's/@''GNULIB_CONNECT''@/$(GNULIB_CONNECT)/g' \ -e 's/@''GNULIB_ACCEPT''@/$(GNULIB_ACCEPT)/g' \ -e 's/@''GNULIB_BIND''@/$(GNULIB_BIND)/g' \ -e 's/@''GNULIB_GETPEERNAME''@/$(GNULIB_GETPEERNAME)/g' \ -e 's/@''GNULIB_GETSOCKNAME''@/$(GNULIB_GETSOCKNAME)/g' \ -e 's/@''GNULIB_GETSOCKOPT''@/$(GNULIB_GETSOCKOPT)/g' \ -e 's/@''GNULIB_LISTEN''@/$(GNULIB_LISTEN)/g' \ -e 's/@''GNULIB_RECV''@/$(GNULIB_RECV)/g' \ -e 's/@''GNULIB_SEND''@/$(GNULIB_SEND)/g' \ -e 's/@''GNULIB_RECVFROM''@/$(GNULIB_RECVFROM)/g' \ -e 's/@''GNULIB_SENDTO''@/$(GNULIB_SENDTO)/g' \ -e 's/@''GNULIB_SETSOCKOPT''@/$(GNULIB_SETSOCKOPT)/g' \ -e 's/@''GNULIB_SHUTDOWN''@/$(GNULIB_SHUTDOWN)/g' \ -e 's/@''GNULIB_ACCEPT4''@/$(GNULIB_ACCEPT4)/g' \ -e 's|@''HAVE_WINSOCK2_H''@|$(HAVE_WINSOCK2_H)|g' \ -e 's|@''HAVE_WS2TCPIP_H''@|$(HAVE_WS2TCPIP_H)|g' \ -e 's|@''HAVE_STRUCT_SOCKADDR_STORAGE''@|$(HAVE_STRUCT_SOCKADDR_STORAGE)|g' \ -e 's|@''HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY''@|$(HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY)|g' \ -e 's|@''HAVE_SA_FAMILY_T''@|$(HAVE_SA_FAMILY_T)|g' \ -e 's|@''HAVE_ACCEPT4''@|$(HAVE_ACCEPT4)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_socket.in.h; \ } > $@-t && \ mv -f $@-t $@ MOSTLYCLEANFILES += sys/socket.h sys/socket.h-t MOSTLYCLEANDIRS += sys EXTRA_DIST += sys_socket.in.h ## end gnulib module sys_socket ## begin gnulib module sys_socket-tests TESTS += test-sys_socket check_PROGRAMS += test-sys_socket EXTRA_DIST += test-sys_socket.c ## end gnulib module sys_socket-tests ## begin gnulib module sys_stat BUILT_SOURCES += sys/stat.h # We need the following in order to create when the system # has one that is incomplete. sys/stat.h: sys_stat.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_STAT_H''@|$(NEXT_SYS_STAT_H)|g' \ -e 's|@''WINDOWS_64_BIT_ST_SIZE''@|$(WINDOWS_64_BIT_ST_SIZE)|g' \ -e 's|@''WINDOWS_STAT_TIMESPEC''@|$(WINDOWS_STAT_TIMESPEC)|g' \ -e 's/@''GNULIB_FCHMODAT''@/$(GNULIB_FCHMODAT)/g' \ -e 's/@''GNULIB_FSTAT''@/$(GNULIB_FSTAT)/g' \ -e 's/@''GNULIB_FSTATAT''@/$(GNULIB_FSTATAT)/g' \ -e 's/@''GNULIB_FUTIMENS''@/$(GNULIB_FUTIMENS)/g' \ -e 's/@''GNULIB_LCHMOD''@/$(GNULIB_LCHMOD)/g' \ -e 's/@''GNULIB_LSTAT''@/$(GNULIB_LSTAT)/g' \ -e 's/@''GNULIB_MKDIRAT''@/$(GNULIB_MKDIRAT)/g' \ -e 's/@''GNULIB_MKFIFO''@/$(GNULIB_MKFIFO)/g' \ -e 's/@''GNULIB_MKFIFOAT''@/$(GNULIB_MKFIFOAT)/g' \ -e 's/@''GNULIB_MKNOD''@/$(GNULIB_MKNOD)/g' \ -e 's/@''GNULIB_MKNODAT''@/$(GNULIB_MKNODAT)/g' \ -e 's/@''GNULIB_STAT''@/$(GNULIB_STAT)/g' \ -e 's/@''GNULIB_UTIMENSAT''@/$(GNULIB_UTIMENSAT)/g' \ -e 's/@''GNULIB_OVERRIDES_STRUCT_STAT''@/$(GNULIB_OVERRIDES_STRUCT_STAT)/g' \ -e 's|@''HAVE_FCHMODAT''@|$(HAVE_FCHMODAT)|g' \ -e 's|@''HAVE_FSTATAT''@|$(HAVE_FSTATAT)|g' \ -e 's|@''HAVE_FUTIMENS''@|$(HAVE_FUTIMENS)|g' \ -e 's|@''HAVE_LCHMOD''@|$(HAVE_LCHMOD)|g' \ -e 's|@''HAVE_LSTAT''@|$(HAVE_LSTAT)|g' \ -e 's|@''HAVE_MKDIRAT''@|$(HAVE_MKDIRAT)|g' \ -e 's|@''HAVE_MKFIFO''@|$(HAVE_MKFIFO)|g' \ -e 's|@''HAVE_MKFIFOAT''@|$(HAVE_MKFIFOAT)|g' \ -e 's|@''HAVE_MKNOD''@|$(HAVE_MKNOD)|g' \ -e 's|@''HAVE_MKNODAT''@|$(HAVE_MKNODAT)|g' \ -e 's|@''HAVE_UTIMENSAT''@|$(HAVE_UTIMENSAT)|g' \ -e 's|@''REPLACE_FSTAT''@|$(REPLACE_FSTAT)|g' \ -e 's|@''REPLACE_FSTATAT''@|$(REPLACE_FSTATAT)|g' \ -e 's|@''REPLACE_FUTIMENS''@|$(REPLACE_FUTIMENS)|g' \ -e 's|@''REPLACE_LSTAT''@|$(REPLACE_LSTAT)|g' \ -e 's|@''REPLACE_MKDIR''@|$(REPLACE_MKDIR)|g' \ -e 's|@''REPLACE_MKFIFO''@|$(REPLACE_MKFIFO)|g' \ -e 's|@''REPLACE_MKNOD''@|$(REPLACE_MKNOD)|g' \ -e 's|@''REPLACE_STAT''@|$(REPLACE_STAT)|g' \ -e 's|@''REPLACE_UTIMENSAT''@|$(REPLACE_UTIMENSAT)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_stat.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/stat.h sys/stat.h-t MOSTLYCLEANDIRS += sys EXTRA_DIST += sys_stat.in.h ## end gnulib module sys_stat ## begin gnulib module sys_stat-tests TESTS += test-sys_stat check_PROGRAMS += test-sys_stat EXTRA_DIST += test-sys_stat.c ## end gnulib module sys_stat-tests ## begin gnulib module sys_time BUILT_SOURCES += sys/time.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/time.h: sys_time.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_SYS_TIME_H''@/$(HAVE_SYS_TIME_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_TIME_H''@|$(NEXT_SYS_TIME_H)|g' \ -e 's/@''GNULIB_GETTIMEOFDAY''@/$(GNULIB_GETTIMEOFDAY)/g' \ -e 's|@''HAVE_WINSOCK2_H''@|$(HAVE_WINSOCK2_H)|g' \ -e 's/@''HAVE_GETTIMEOFDAY''@/$(HAVE_GETTIMEOFDAY)/g' \ -e 's/@''HAVE_STRUCT_TIMEVAL''@/$(HAVE_STRUCT_TIMEVAL)/g' \ -e 's/@''REPLACE_GETTIMEOFDAY''@/$(REPLACE_GETTIMEOFDAY)/g' \ -e 's/@''REPLACE_STRUCT_TIMEVAL''@/$(REPLACE_STRUCT_TIMEVAL)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/sys_time.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/time.h sys/time.h-t EXTRA_DIST += sys_time.in.h ## end gnulib module sys_time ## begin gnulib module sys_time-tests TESTS += test-sys_time check_PROGRAMS += test-sys_time EXTRA_DIST += test-sys_time.c ## end gnulib module sys_time-tests ## begin gnulib module sys_types-tests TESTS += test-sys_types check_PROGRAMS += test-sys_types EXTRA_DIST += test-sys_types.c ## end gnulib module sys_types-tests ## begin gnulib module sys_uio BUILT_SOURCES += sys/uio.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/uio.h: sys_uio.in.h $(top_builddir)/config.status $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_UIO_H''@|$(NEXT_SYS_UIO_H)|g' \ -e 's|@''HAVE_SYS_UIO_H''@|$(HAVE_SYS_UIO_H)|g' \ < $(srcdir)/sys_uio.in.h; \ } > $@-t && \ mv -f $@-t $@ MOSTLYCLEANFILES += sys/uio.h sys/uio.h-t MOSTLYCLEANDIRS += sys EXTRA_DIST += sys_uio.in.h ## end gnulib module sys_uio ## begin gnulib module sys_uio-tests TESTS += test-sys_uio check_PROGRAMS += test-sys_uio EXTRA_DIST += test-sys_uio.c ## end gnulib module sys_uio-tests ## begin gnulib module sysexits-tests TESTS += test-sysexits check_PROGRAMS += test-sysexits EXTRA_DIST += test-sysexits.c ## end gnulib module sysexits-tests ## begin gnulib module test-framework-sh-tests TESTS += test-init.sh EXTRA_DIST += init.sh EXTRA_DIST += test-init.sh ## end gnulib module test-framework-sh-tests ## begin gnulib module thread libtests_a_SOURCES += glthread/thread.h glthread/thread.c ## end gnulib module thread ## begin gnulib module thread-tests TESTS += test-thread_self test-thread_create check_PROGRAMS += test-thread_self test-thread_create test_thread_self_LDADD = $(LDADD) @LIBTHREAD@ test_thread_create_LDADD = $(LDADD) @LIBMULTITHREAD@ EXTRA_DIST += test-thread_self.c test-thread_create.c macros.h ## end gnulib module thread-tests ## begin gnulib module time BUILT_SOURCES += time.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. time.h: time.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_TIME_H''@|$(NEXT_TIME_H)|g' \ -e 's/@''GNULIB_CTIME''@/$(GNULIB_CTIME)/g' \ -e 's/@''GNULIB_LOCALTIME''@/$(GNULIB_LOCALTIME)/g' \ -e 's/@''GNULIB_MKTIME''@/$(GNULIB_MKTIME)/g' \ -e 's/@''GNULIB_NANOSLEEP''@/$(GNULIB_NANOSLEEP)/g' \ -e 's/@''GNULIB_STRFTIME''@/$(GNULIB_STRFTIME)/g' \ -e 's/@''GNULIB_STRPTIME''@/$(GNULIB_STRPTIME)/g' \ -e 's/@''GNULIB_TIMEGM''@/$(GNULIB_TIMEGM)/g' \ -e 's/@''GNULIB_TIME_R''@/$(GNULIB_TIME_R)/g' \ -e 's/@''GNULIB_TIME_RZ''@/$(GNULIB_TIME_RZ)/g' \ -e 's/@''GNULIB_TZSET''@/$(GNULIB_TZSET)/g' \ -e 's|@''HAVE_DECL_LOCALTIME_R''@|$(HAVE_DECL_LOCALTIME_R)|g' \ -e 's|@''HAVE_NANOSLEEP''@|$(HAVE_NANOSLEEP)|g' \ -e 's|@''HAVE_STRPTIME''@|$(HAVE_STRPTIME)|g' \ -e 's|@''HAVE_TIMEGM''@|$(HAVE_TIMEGM)|g' \ -e 's|@''HAVE_TIMEZONE_T''@|$(HAVE_TIMEZONE_T)|g' \ -e 's|@''HAVE_TZSET''@|$(HAVE_TZSET)|g' \ -e 's|@''REPLACE_CTIME''@|$(REPLACE_CTIME)|g' \ -e 's|@''REPLACE_GMTIME''@|$(REPLACE_GMTIME)|g' \ -e 's|@''REPLACE_LOCALTIME''@|$(REPLACE_LOCALTIME)|g' \ -e 's|@''REPLACE_LOCALTIME_R''@|$(REPLACE_LOCALTIME_R)|g' \ -e 's|@''REPLACE_MKTIME''@|$(REPLACE_MKTIME)|g' \ -e 's|@''REPLACE_NANOSLEEP''@|$(REPLACE_NANOSLEEP)|g' \ -e 's|@''REPLACE_STRFTIME''@|$(REPLACE_STRFTIME)|g' \ -e 's|@''REPLACE_TIMEGM''@|$(REPLACE_TIMEGM)|g' \ -e 's|@''REPLACE_TZSET''@|$(REPLACE_TZSET)|g' \ -e 's|@''PTHREAD_H_DEFINES_STRUCT_TIMESPEC''@|$(PTHREAD_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e 's|@''SYS_TIME_H_DEFINES_STRUCT_TIMESPEC''@|$(SYS_TIME_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e 's|@''TIME_H_DEFINES_STRUCT_TIMESPEC''@|$(TIME_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e 's|@''UNISTD_H_DEFINES_STRUCT_TIMESPEC''@|$(UNISTD_H_DEFINES_STRUCT_TIMESPEC)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/time.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += time.h time.h-t EXTRA_DIST += time.in.h ## end gnulib module time ## begin gnulib module time-tests TESTS += test-time check_PROGRAMS += test-time EXTRA_DIST += test-time.c ## end gnulib module time-tests ## begin gnulib module unistd-tests TESTS += test-unistd check_PROGRAMS += test-unistd EXTRA_DIST += test-unistd.c ## end gnulib module unistd-tests ## begin gnulib module uniwidth/width-tests TESTS += test-uc_width uniwidth/test-uc_width2.sh check_PROGRAMS += test-uc_width test-uc_width2 test_uc_width_SOURCES = uniwidth/test-uc_width.c test_uc_width_LDADD = $(LDADD) $(LIBUNISTRING) test_uc_width2_SOURCES = uniwidth/test-uc_width2.c test_uc_width2_LDADD = $(LDADD) $(LIBUNISTRING) EXTRA_DIST += uniwidth/test-uc_width.c uniwidth/test-uc_width2.c uniwidth/test-uc_width2.sh macros.h ## end gnulib module uniwidth/width-tests ## begin gnulib module unsetenv EXTRA_DIST += unsetenv.c EXTRA_libtests_a_SOURCES += unsetenv.c ## end gnulib module unsetenv ## begin gnulib module unsetenv-tests TESTS += test-unsetenv check_PROGRAMS += test-unsetenv EXTRA_DIST += test-unsetenv.c signature.h macros.h ## end gnulib module unsetenv-tests ## begin gnulib module usleep EXTRA_DIST += usleep.c EXTRA_libtests_a_SOURCES += usleep.c ## end gnulib module usleep ## begin gnulib module usleep-tests TESTS += test-usleep check_PROGRAMS += test-usleep EXTRA_DIST += test-usleep.c signature.h macros.h ## end gnulib module usleep-tests ## begin gnulib module vasnprintf-tests TESTS += test-vasnprintf check_PROGRAMS += test-vasnprintf EXTRA_DIST += test-vasnprintf.c macros.h ## end gnulib module vasnprintf-tests ## begin gnulib module verify-tests TESTS_ENVIRONMENT += MAKE='$(MAKE)' TESTS += test-verify test-verify.sh check_PROGRAMS += test-verify # test-verify-try is never built, but test-verify.sh needs a rule to # build test-verify-try.o. EXTRA_PROGRAMS += test-verify-try # This test expects compilation of test-verify-try.c to fail, and # each time it fails, the makefile rule does not perform the usual # "mv -f $name.Tpo $name.po, so tell make clean to remove that file. MOSTLYCLEANFILES += .deps/test-verify-try.Tpo EXTRA_DIST += test-verify.c test-verify-try.c test-verify.sh ## end gnulib module verify-tests ## begin gnulib module vsnprintf-tests TESTS += test-vsnprintf check_PROGRAMS += test-vsnprintf EXTRA_DIST += test-vsnprintf.c signature.h macros.h ## end gnulib module vsnprintf-tests ## begin gnulib module wchar-tests TESTS += test-wchar check_PROGRAMS += test-wchar EXTRA_DIST += test-wchar.c ## end gnulib module wchar-tests ## begin gnulib module wcrtomb-tests TESTS += \ test-wcrtomb.sh \ test-wcrtomb-w32-1.sh test-wcrtomb-w32-2.sh test-wcrtomb-w32-3.sh \ test-wcrtomb-w32-4.sh test-wcrtomb-w32-5.sh TESTS_ENVIRONMENT += \ LOCALE_FR='@LOCALE_FR@' \ LOCALE_FR_UTF8='@LOCALE_FR_UTF8@' \ LOCALE_JA='@LOCALE_JA@' \ LOCALE_ZH_CN='@LOCALE_ZH_CN@' check_PROGRAMS += test-wcrtomb test-wcrtomb-w32 EXTRA_DIST += test-wcrtomb.sh test-wcrtomb.c test-wcrtomb-w32-1.sh test-wcrtomb-w32-2.sh test-wcrtomb-w32-3.sh test-wcrtomb-w32-4.sh test-wcrtomb-w32-5.sh test-wcrtomb-w32.c signature.h macros.h ## end gnulib module wcrtomb-tests ## begin gnulib module wctob EXTRA_DIST += wctob.c EXTRA_libtests_a_SOURCES += wctob.c ## end gnulib module wctob ## begin gnulib module wctomb EXTRA_DIST += wctomb-impl.h wctomb.c EXTRA_libtests_a_SOURCES += wctomb.c ## end gnulib module wctomb ## begin gnulib module wctype-h-tests TESTS += test-wctype-h check_PROGRAMS += test-wctype-h EXTRA_DIST += test-wctype-h.c macros.h ## end gnulib module wctype-h-tests ## begin gnulib module wcwidth-tests TESTS += test-wcwidth check_PROGRAMS += test-wcwidth EXTRA_DIST += test-wcwidth.c signature.h macros.h ## end gnulib module wcwidth-tests ## begin gnulib module xalloc-oversized EXTRA_DIST += xalloc-oversized.h ## end gnulib module xalloc-oversized ## begin gnulib module yield libtests_a_SOURCES += glthread/yield.h ## end gnulib module yield # Clean up after Solaris cc. clean-local: rm -rf SunWS_cache mostlyclean-local: mostlyclean-generic @for dir in '' $(MOSTLYCLEANDIRS); do \ if test -n "$$dir" && test -d $$dir; then \ echo "rmdir $$dir"; rmdir $$dir; \ fi; \ done; \ : gnuastro-0.5/bootstrapped/tests/uniwidth/0000755000175000017500000000000013217220466015727 500000000000000gnuastro-0.5/bootstrapped/tests/uniwidth/test-uc_width2.sh0000755000175000017500000001715113217200024021044 00000000000000#!/bin/sh tmpfiles="" trap 'rm -fr $tmpfiles' 1 2 3 15 tmpfiles="$tmpfiles uc_width.out" ./test-uc_width2${EXEEXT} | LC_ALL=C tr -d '\r' > uc_width.out tmpfiles="$tmpfiles uc_width.ok" cat > uc_width.ok <<\EOF 0000 0 0020..007E 1 00A0 1 00A1..00AC A 00AD 0 00AE..02FF A 0300..036F 0 0370..0482 A 0483..0489 0 048A..0590 A 0591..05BD 0 05BE A 05BF 0 05C0 A 05C1..05C2 0 05C3 A 05C4..05C5 0 05C6 A 05C7 0 05C8..05FF A 0600..0605 0 0606..060F A 0610..061A 0 061B A 061C 0 061D..064A A 064B..065F 0 0660..066F A 0670 0 0671..06D5 A 06D6..06DD 0 06DE A 06DF..06E4 0 06E5..06E6 A 06E7..06E8 0 06E9 A 06EA..06ED 0 06EE..070E A 070F 0 0710 A 0711 0 0712..072F A 0730..074A 0 074B..07A5 A 07A6..07B0 0 07B1..07EA A 07EB..07F3 0 07F4..0815 A 0816..0819 0 081A A 081B..0823 0 0824 A 0825..0827 0 0828 A 0829..082D 0 082E..0858 A 0859..085B 0 085C..08D3 A 08D4..0902 0 0903..0939 A 093A 0 093B A 093C 0 093D..0940 A 0941..0948 0 0949..094C A 094D 0 094E..0950 A 0951..0957 0 0958..0961 A 0962..0963 0 0964..0980 A 0981 0 0982..09BB A 09BC 0 09BD..09C0 A 09C1..09C4 0 09C5..09CC A 09CD 0 09CE..09E1 A 09E2..09E3 0 09E4..0A00 A 0A01..0A02 0 0A03..0A3B A 0A3C 0 0A3D..0A40 A 0A41..0A42 0 0A43..0A46 A 0A47..0A48 0 0A49..0A4A A 0A4B..0A4D 0 0A4E..0A50 A 0A51 0 0A52..0A6F A 0A70..0A71 0 0A72..0A74 A 0A75 0 0A76..0A80 A 0A81..0A82 0 0A83..0ABB A 0ABC 0 0ABD..0AC0 A 0AC1..0AC5 0 0AC6 A 0AC7..0AC8 0 0AC9..0ACC A 0ACD 0 0ACE..0AE1 A 0AE2..0AE3 0 0AE4..0B00 A 0B01 0 0B02..0B3B A 0B3C 0 0B3D..0B3E A 0B3F 0 0B40 A 0B41..0B44 0 0B45..0B4C A 0B4D 0 0B4E..0B55 A 0B56 0 0B57..0B61 A 0B62..0B63 0 0B64..0B81 A 0B82 0 0B83..0BBF A 0BC0 0 0BC1..0BCC A 0BCD 0 0BCE..0BFF A 0C00 0 0C01..0C3D A 0C3E..0C40 0 0C41..0C45 A 0C46..0C48 0 0C49 A 0C4A..0C4D 0 0C4E..0C54 A 0C55..0C56 0 0C57..0C61 A 0C62..0C63 0 0C64..0C80 A 0C81 0 0C82..0CBB A 0CBC 0 0CBD..0CCB A 0CCC..0CCD 0 0CCE..0CE1 A 0CE2..0CE3 0 0CE4..0D00 A 0D01 0 0D02..0D40 A 0D41..0D44 0 0D45..0D4C A 0D4D 0 0D4E..0D61 A 0D62..0D63 0 0D64..0DC9 A 0DCA 0 0DCB..0DD1 A 0DD2..0DD4 0 0DD5 A 0DD6 0 0DD7..0E30 A 0E31 0 0E32..0E33 A 0E34..0E3A 0 0E3B..0E46 A 0E47..0E4E 0 0E4F..0EB0 A 0EB1 0 0EB2..0EB3 A 0EB4..0EB9 0 0EBA A 0EBB..0EBC 0 0EBD..0EC7 A 0EC8..0ECD 0 0ECE..0F17 A 0F18..0F19 0 0F1A..0F34 A 0F35 0 0F36 A 0F37 0 0F38 A 0F39 0 0F3A..0F70 A 0F71..0F7E 0 0F7F A 0F80..0F84 0 0F85 A 0F86..0F87 0 0F88..0F8C A 0F8D..0F97 0 0F98 A 0F99..0FBC 0 0FBD..0FC5 A 0FC6 0 0FC7..102C A 102D..1030 0 1031 A 1032..1037 0 1038 A 1039..103A 0 103B..103C A 103D..103E 0 103F..1057 A 1058..1059 0 105A..105D A 105E..1060 0 1061..1070 A 1071..1074 0 1075..1081 A 1082 0 1083..1084 A 1085..1086 0 1087..108C A 108D 0 108E..109C A 109D 0 109E..10FF A 1100..115F 2 1160..135C A 135D..135F 0 1360..1711 A 1712..1714 0 1715..1731 A 1732..1734 0 1735..1751 A 1752..1753 0 1754..1771 A 1772..1773 0 1774..17B3 A 17B4..17B5 0 17B6 A 17B7..17BD 0 17BE..17C5 A 17C6 0 17C7..17C8 A 17C9..17D3 0 17D4..17DC A 17DD 0 17DE..180A A 180B..180E 0 180F..1884 A 1885..1886 0 1887..18A8 A 18A9 0 18AA..191F A 1920..1922 0 1923..1926 A 1927..1928 0 1929..1931 A 1932 0 1933..1938 A 1939..193B 0 193C..1A16 A 1A17..1A18 0 1A19..1A1A A 1A1B 0 1A1C..1A55 A 1A56 0 1A57 A 1A58..1A5E 0 1A5F A 1A60 0 1A61 A 1A62 0 1A63..1A64 A 1A65..1A6C 0 1A6D..1A72 A 1A73..1A7C 0 1A7D..1A7E A 1A7F 0 1A80..1AAF A 1AB0..1ABE 0 1ABF..1AFF A 1B00..1B03 0 1B04..1B33 A 1B34 0 1B35 A 1B36..1B3A 0 1B3B A 1B3C 0 1B3D..1B41 A 1B42 0 1B43..1B6A A 1B6B..1B73 0 1B74..1B7F A 1B80..1B81 0 1B82..1BA1 A 1BA2..1BA5 0 1BA6..1BA7 A 1BA8..1BA9 0 1BAA A 1BAB..1BAD 0 1BAE..1BE5 A 1BE6 0 1BE7 A 1BE8..1BE9 0 1BEA..1BEC A 1BED 0 1BEE A 1BEF..1BF1 0 1BF2..1C2B A 1C2C..1C33 0 1C34..1C35 A 1C36..1C37 0 1C38..1CCF A 1CD0..1CD2 0 1CD3 A 1CD4..1CE0 0 1CE1 A 1CE2..1CE8 0 1CE9..1CEC A 1CED 0 1CEE..1CF3 A 1CF4 0 1CF5..1CF7 A 1CF8..1CF9 0 1CFA..1DBF A 1DC0..1DF5 0 1DF6..1DFA A 1DFB..1DFF 0 1E00..200A A 200B..200F 0 2010..2029 A 202A..202E 0 202F..205F A 2060..2064 0 2065 A 2066..206F 0 2070..20A8 A 20A9 1 20AA..20CF A 20D0..20F0 0 20F1..2328 A 2329..232A 2 232B..2CEE A 2CEF..2CF1 0 2CF2..2D7E A 2D7F 0 2D80..2DDF A 2DE0..2DFF 0 2E00..2E7F A 2E80..3029 2 302A..302D 0 302E..303E 2 303F A 3040..3098 2 3099..309A 0 309B..4DBF 2 4DC0..4DFF A 4E00..A4CF 2 A4D0..A66E A A66F..A672 0 A673 A A674..A67D 0 A67E..A69D A A69E..A69F 0 A6A0..A6EF A A6F0..A6F1 0 A6F2..A801 A A802 0 A803..A805 A A806 0 A807..A80A A A80B 0 A80C..A824 A A825..A826 0 A827..A8C3 A A8C4..A8C5 0 A8C6..A8DF A A8E0..A8F1 0 A8F2..A925 A A926..A92D 0 A92E..A946 A A947..A951 0 A952..A97F A A980..A982 0 A983..A9B2 A A9B3 0 A9B4..A9B5 A A9B6..A9B9 0 A9BA..A9BB A A9BC 0 A9BD..A9E4 A A9E5 0 A9E6..AA28 A AA29..AA2E 0 AA2F..AA30 A AA31..AA32 0 AA33..AA34 A AA35..AA36 0 AA37..AA42 A AA43 0 AA44..AA4B A AA4C 0 AA4D..AA7B A AA7C 0 AA7D..AAAF A AAB0 0 AAB1 A AAB2..AAB4 0 AAB5..AAB6 A AAB7..AAB8 0 AAB9..AABD A AABE..AABF 0 AAC0 A AAC1 0 AAC2..AAEB A AAEC..AAED 0 AAEE..AAF5 A AAF6 0 AAF7..ABE4 A ABE5 0 ABE6..ABE7 A ABE8 0 ABE9..ABEC A ABED 0 ABEE..ABFF A AC00..D7A3 2 D7A4..F8FF A F900..FAFF 2 FB00..FB1D A FB1E 0 FB1F..FDFF A FE00..FE0F 0 FE10..FE1F 2 FE20..FE2F 0 FE30..FE6F 2 FE70..FEFE A FEFF 0 FF00..FF60 2 FF61..FFDF 1 FFE0..FFE6 2 FFE7..FFF8 1 FFF9..FFFB 0 FFFC..101FC 1 101FD 0 101FE..102DF 1 102E0 0 102E1..10375 1 10376..1037A 0 1037B..10A00 1 10A01..10A03 0 10A04 1 10A05..10A06 0 10A07..10A0B 1 10A0C..10A0F 0 10A10..10A37 1 10A38..10A3A 0 10A3B..10A3E 1 10A3F 0 10A40..10AE4 1 10AE5..10AE6 0 10AE7..11000 1 11001 0 11002..11037 1 11038..11046 0 11047..1107E 1 1107F..11081 0 11082..110B2 1 110B3..110B6 0 110B7..110B8 1 110B9..110BA 0 110BB..110BC 1 110BD 0 110BE..110FF 1 11100..11102 0 11103..11126 1 11127..1112B 0 1112C 1 1112D..11134 0 11135..11172 1 11173 0 11174..1117F 1 11180..11181 0 11182..111B5 1 111B6..111BE 0 111BF..111C9 1 111CA..111CC 0 111CD..1122E 1 1122F..11231 0 11232..11233 1 11234 0 11235 1 11236..11237 0 11238..1123D 1 1123E 0 1123F..112DE 1 112DF 0 112E0..112E2 1 112E3..112EA 0 112EB..112FF 1 11300..11301 0 11302..1133B 1 1133C 0 1133D..1133F 1 11340 0 11341..11365 1 11366..1136C 0 1136D..1136F 1 11370..11374 0 11375..11437 1 11438..1143F 0 11440..11441 1 11442..11444 0 11445 1 11446 0 11447..114B2 1 114B3..114B8 0 114B9 1 114BA 0 114BB..114BE 1 114BF..114C0 0 114C1 1 114C2..114C3 0 114C4..115B1 1 115B2..115B5 0 115B6..115BB 1 115BC..115BD 0 115BE 1 115BF..115C0 0 115C1..115DB 1 115DC..115DD 0 115DE..11632 1 11633..1163A 0 1163B..1163C 1 1163D 0 1163E 1 1163F..11640 0 11641..116AA 1 116AB 0 116AC 1 116AD 0 116AE..116AF 1 116B0..116B5 0 116B6 1 116B7 0 116B8..1171C 1 1171D..1171F 0 11720..11721 1 11722..11725 0 11726 1 11727..1172B 0 1172C..11C2F 1 11C30..11C36 0 11C37 1 11C38..11C3D 0 11C3E..11C91 1 11C92..11CA7 0 11CA8..11CA9 1 11CAA..11CB0 0 11CB1 1 11CB2..11CB3 0 11CB4 1 11CB5..11CB6 0 11CB7..16AEF 1 16AF0..16AF4 0 16AF5..16B2F 1 16B30..16B36 0 16B37..16F8E 1 16F8F..16F92 0 16F93..1BC9C 1 1BC9D..1BC9E 0 1BC9F 1 1BCA0..1BCA3 0 1BCA4..1D166 1 1D167..1D169 0 1D16A..1D172 1 1D173..1D182 0 1D183..1D184 1 1D185..1D18B 0 1D18C..1D1A9 1 1D1AA..1D1AD 0 1D1AE..1D241 1 1D242..1D244 0 1D245..1D9FF 1 1DA00..1DA36 0 1DA37..1DA3A 1 1DA3B..1DA6C 0 1DA6D..1DA74 1 1DA75 0 1DA76..1DA83 1 1DA84 0 1DA85..1DA9A 1 1DA9B..1DA9F 0 1DAA0 1 1DAA1..1DAAF 0 1DAB0..1DFFF 1 1E000..1E006 0 1E007 1 1E008..1E018 0 1E019..1E01A 1 1E01B..1E021 0 1E022 1 1E023..1E024 0 1E025 1 1E026..1E02A 0 1E02B..1E8CF 1 1E8D0..1E8D6 0 1E8D7..1E943 1 1E944..1E94A 0 1E94B..1FFFF 1 20000..3FFFF 2 40000..E0000 1 E0001 0 E0002..E001F 1 E0020..E007F 0 E0080..E00FF 1 E0100..E01EF 0 E01F0..10FFFF 1 EOF : ${DIFF=diff} ${DIFF} uc_width.ok uc_width.out result=$? rm -fr $tmpfiles exit $result gnuastro-0.5/bootstrapped/tests/uniwidth/test-uc_width2.c0000644000175000017500000000422013217200024020642 00000000000000/* Test of uc_width() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2008. */ #include #include "uniwidth.h" #include #include "macros.h" /* One of 0, '0', '1', 'A', '2'. */ static char current_width; /* The interval for which the current_width holds. */ static ucs4_t current_start; static ucs4_t current_end; static void finish_interval (void) { if (current_width != 0) { if (current_start == current_end) printf ("%04X\t\t%c\n", (unsigned) current_start, current_width); else printf ("%04X..%04X\t%c\n", (unsigned) current_start, (unsigned) current_end, current_width); current_width = 0; } } static void add_to_interval (ucs4_t uc, char width) { if (current_width == width && uc == current_end + 1) current_end = uc; else { finish_interval (); current_width = width; current_start = current_end = uc; } } int main () { ucs4_t uc; for (uc = 0; uc < 0x110000; uc++) { int w1 = uc_width (uc, "UTF-8"); int w2 = uc_width (uc, "GBK"); char width = (w1 == 0 && w2 == 0 ? '0' : w1 == 1 && w2 == 1 ? '1' : w1 == 1 && w2 == 2 ? 'A' : w1 == 2 && w2 == 2 ? '2' : 0); if (width == 0) { /* uc must be a control character. */ ASSERT (w1 < 0 && w2 < 0); } else add_to_interval (uc, width); } finish_interval (); return 0; } gnuastro-0.5/bootstrapped/tests/uniwidth/test-uc_width.c0000644000175000017500000000342513217200024020566 00000000000000/* Test of uc_width() function. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2007. */ #include #include "uniwidth.h" #include "macros.h" int main () { ucs4_t uc; /* Test width of ASCII characters. */ for (uc = 0x0020; uc < 0x007F; uc++) ASSERT (uc_width (uc, "ISO-8859-2") == 1); /* Test width of some non-spacing characters. */ ASSERT (uc_width (0x0301, "UTF-8") == 0); ASSERT (uc_width (0x05B0, "UTF-8") == 0); /* Test width of some format control characters. */ ASSERT (uc_width (0x200E, "UTF-8") == 0); ASSERT (uc_width (0x2060, "UTF-8") == 0); ASSERT (uc_width (0xE0001, "UTF-8") == 0); ASSERT (uc_width (0xE0044, "UTF-8") == 0); /* Test width of some zero width characters. */ ASSERT (uc_width (0x200B, "UTF-8") == 0); ASSERT (uc_width (0xFEFF, "UTF-8") == 0); /* Test width of some CJK characters. */ ASSERT (uc_width (0x3000, "UTF-8") == 2); ASSERT (uc_width (0xB250, "UTF-8") == 2); ASSERT (uc_width (0xFF1A, "UTF-8") == 2); ASSERT (uc_width (0x20369, "UTF-8") == 2); ASSERT (uc_width (0x2F876, "UTF-8") == 2); return 0; } gnuastro-0.5/bootstrapped/tests/glthread/0000755000175000017500000000000013217220465015665 500000000000000gnuastro-0.5/bootstrapped/tests/glthread/yield.h0000644000175000017500000000475013217200022017055 00000000000000/* Yielding the processor to other threads and processes. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file contains a primitive for yielding the processor to other threads. extern void gl_thread_yield (void); */ #ifndef _GLTHREAD_YIELD_H #define _GLTHREAD_YIELD_H #include /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ sched_yield () # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ pth_yield (NULL) # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ thr_yield () # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # ifdef __cplusplus extern "C" { # endif # define gl_thread_yield() \ Sleep (0) # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if !(USE_POSIX_THREADS || USE_PTH_THREADS || USE_SOLARIS_THREADS || USE_WINDOWS_THREADS) /* Provide dummy implementation if threads are not supported. */ # define gl_thread_yield() 0 #endif /* ========================================================================= */ #endif /* _GLTHREAD_YIELD_H */ gnuastro-0.5/bootstrapped/tests/glthread/thread.c0000644000175000017500000001427413217200022017213 00000000000000/* Creating and controlling threads. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ #include /* Specification. */ # define _GLTHREAD_THREAD_INLINE _GL_EXTERN_INLINE #include "glthread/thread.h" #include #include "glthread/lock.h" /* ========================================================================= */ #if USE_POSIX_THREADS #include #if defined PTW32_VERSION || defined __MVS__ const gl_thread_t gl_null_thread /* = { .p = NULL } */; #endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS #include /* -------------------------- gl_thread_t datatype -------------------------- */ /* The Thread-Local Storage (TLS) key that allows to access each thread's 'struct gl_thread_struct *' pointer. */ static DWORD self_key = (DWORD)-1; /* Initializes self_key. This function must only be called once. */ static void do_init_self_key (void) { self_key = TlsAlloc (); /* If this fails, we're hosed. */ if (self_key == (DWORD)-1) abort (); } /* Initializes self_key. */ static void init_self_key (void) { gl_once_define(static, once) gl_once (once, do_init_self_key); } /* This structure contains information about a thread. It is stored in TLS under key self_key. */ struct gl_thread_struct { /* Fields for managing the handle. */ HANDLE volatile handle; CRITICAL_SECTION handle_lock; /* Fields for managing the exit value. */ void * volatile result; /* Fields for managing the thread start. */ void * (*func) (void *); void *arg; }; /* Return a real HANDLE object for the current thread. */ static HANDLE get_current_thread_handle (void) { HANDLE this_handle; /* GetCurrentThread() returns a pseudo-handle, i.e. only a symbolic identifier, not a real handle. */ if (!DuplicateHandle (GetCurrentProcess (), GetCurrentThread (), GetCurrentProcess (), &this_handle, 0, FALSE, DUPLICATE_SAME_ACCESS)) abort (); return this_handle; } gl_thread_t gl_thread_self_func (void) { gl_thread_t thread; if (self_key == (DWORD)-1) init_self_key (); thread = TlsGetValue (self_key); if (thread == NULL) { /* This happens only in threads that have not been created through glthread_create(), such as the main thread. */ for (;;) { thread = (struct gl_thread_struct *) malloc (sizeof (struct gl_thread_struct)); if (thread != NULL) break; /* Memory allocation failed. There is not much we can do. Have to busy-loop, waiting for the availability of memory. */ Sleep (1); } thread->handle = get_current_thread_handle (); InitializeCriticalSection (&thread->handle_lock); thread->result = NULL; /* just to be deterministic */ TlsSetValue (self_key, thread); } return thread; } /* The main function of a freshly creating thread. It's a wrapper around the FUNC and ARG arguments passed to glthread_create_func. */ static unsigned int WINAPI wrapper_func (void *varg) { struct gl_thread_struct *thread = (struct gl_thread_struct *)varg; EnterCriticalSection (&thread->handle_lock); /* Create a new handle for the thread only if the parent thread did not yet fill in the handle. */ if (thread->handle == NULL) thread->handle = get_current_thread_handle (); LeaveCriticalSection (&thread->handle_lock); if (self_key == (DWORD)-1) init_self_key (); TlsSetValue (self_key, thread); /* Run the thread. Store the exit value if the thread was not terminated otherwise. */ thread->result = thread->func (thread->arg); return 0; } int glthread_create_func (gl_thread_t *threadp, void * (*func) (void *), void *arg) { struct gl_thread_struct *thread = (struct gl_thread_struct *) malloc (sizeof (struct gl_thread_struct)); if (thread == NULL) return ENOMEM; thread->handle = NULL; InitializeCriticalSection (&thread->handle_lock); thread->result = NULL; /* just to be deterministic */ thread->func = func; thread->arg = arg; { unsigned int thread_id; HANDLE thread_handle; thread_handle = (HANDLE) _beginthreadex (NULL, 100000, wrapper_func, thread, 0, &thread_id); /* calls CreateThread with the same arguments */ if (thread_handle == NULL) { DeleteCriticalSection (&thread->handle_lock); free (thread); return EAGAIN; } EnterCriticalSection (&thread->handle_lock); if (thread->handle == NULL) thread->handle = thread_handle; else /* thread->handle was already set by the thread itself. */ CloseHandle (thread_handle); LeaveCriticalSection (&thread->handle_lock); *threadp = thread; return 0; } } int glthread_join_func (gl_thread_t thread, void **retvalp) { if (thread == NULL) return EINVAL; if (thread == gl_thread_self ()) return EDEADLK; if (WaitForSingleObject (thread->handle, INFINITE) == WAIT_FAILED) return EINVAL; if (retvalp != NULL) *retvalp = thread->result; DeleteCriticalSection (&thread->handle_lock); CloseHandle (thread->handle); free (thread); return 0; } int gl_thread_exit_func (void *retval) { gl_thread_t thread = gl_thread_self (); thread->result = retval; _endthreadex (0); /* calls ExitThread (0) */ abort (); } #endif /* ========================================================================= */ gnuastro-0.5/bootstrapped/tests/glthread/thread.h0000644000175000017500000003263513217200022017221 00000000000000/* Creating and controlling threads. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ /* This file contains primitives for creating and controlling threads. Thread data type: gl_thread_t. Creating a thread: thread = gl_thread_create (func, arg); Or with control of error handling: err = glthread_create (&thread, func, arg); extern int glthread_create (gl_thread_t *result, void *(*func) (void *), void *arg); Querying and changing the signal mask of a thread (not supported on all platforms): gl_thread_sigmask (how, newmask, oldmask); Or with control of error handling: err = glthread_sigmask (how, newmask, oldmask); extern int glthread_sigmask (int how, const sigset_t *newmask, sigset_t *oldmask); Waiting for termination of another thread: gl_thread_join (thread, &return_value); Or with control of error handling: err = glthread_join (thread, &return_value); extern int glthread_join (gl_thread_t thread, void **return_value_ptr); Getting a reference to the current thread: current = gl_thread_self (); extern gl_thread_t gl_thread_self (void); Getting a reference to the current thread as a pointer, for debugging: ptr = gl_thread_self_pointer (); extern void * gl_thread_self_pointer (void); Terminating the current thread: gl_thread_exit (return_value); extern _Noreturn void gl_thread_exit (void *return_value); Requesting custom code to be executed at fork() time(not supported on all platforms): gl_thread_atfork (prepare_func, parent_func, child_func); Or with control of error handling: err = glthread_atfork (prepare_func, parent_func, child_func); extern int glthread_atfork (void (*prepare_func) (void), void (*parent_func) (void), void (*child_func) (void)); Note that even on platforms where this is supported, use of fork() and threads together is problematic, see */ #ifndef _GLTHREAD_THREAD_H #define _GLTHREAD_THREAD_H #include #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GLTHREAD_THREAD_INLINE # define _GLTHREAD_THREAD_INLINE _GL_INLINE #endif /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if PTHREAD_IN_USE_DETECTION_HARD /* The pthread_in_use() detection needs to be done at runtime. */ # define pthread_in_use() \ glthread_in_use () extern int glthread_in_use (void); # endif # if USE_POSIX_THREADS_WEAK /* Use weak references to the POSIX threads library. */ /* Weak references avoid dragging in external libraries if the other parts of the program don't use them. Here we use them, because we don't want every program that uses libintl to depend on libpthread. This assumes that libpthread would not be loaded after libintl; i.e. if libintl is loaded first, by an executable that does not depend on libpthread, and then a module is dynamically loaded that depends on libpthread, libintl will not be multithread-safe. */ /* The way to test at runtime whether libpthread is present is to test whether a function pointer's value, such as &pthread_mutex_init, is non-NULL. However, some versions of GCC have a bug through which, in PIC mode, &foo != NULL always evaluates to true if there is a direct call to foo(...) in the same function. To avoid this, we test the address of a function in libpthread that we don't use. */ # pragma weak pthread_create # ifdef __clang__ /* Without this, clang complains that pthread_sigmask is never declared. */ # include # endif # ifndef pthread_sigmask /* Do not declare rpl_pthread_sigmask weak. */ # pragma weak pthread_sigmask # endif # pragma weak pthread_join # ifndef pthread_self # pragma weak pthread_self # endif # pragma weak pthread_exit # if HAVE_PTHREAD_ATFORK # pragma weak pthread_atfork # endif # if !PTHREAD_IN_USE_DETECTION_HARD # pragma weak pthread_cancel # define pthread_in_use() (pthread_cancel != NULL) # endif # else # if !PTHREAD_IN_USE_DETECTION_HARD # define pthread_in_use() 1 # endif # endif /* -------------------------- gl_thread_t datatype -------------------------- */ /* This choice of gl_thread_t assumes that pthread_equal (a, b) is equivalent to ((a) == (b)). This is the case on all platforms in use in 2008. */ typedef pthread_t gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ (pthread_in_use () ? pthread_create (THREADP, NULL, FUNC, ARG) : ENOSYS) # define glthread_sigmask(HOW, SET, OSET) \ (pthread_in_use () ? pthread_sigmask (HOW, SET, OSET) : 0) # define glthread_join(THREAD, RETVALP) \ (pthread_in_use () ? pthread_join (THREAD, RETVALP) : 0) # ifdef PTW32_VERSION /* In pthreads-win32, pthread_t is a struct with a pointer field 'p' and other fields. */ # define gl_thread_self() \ (pthread_in_use () ? pthread_self () : gl_null_thread) # define gl_thread_self_pointer() \ (pthread_in_use () ? pthread_self ().p : NULL) extern const gl_thread_t gl_null_thread; # elif defined __MVS__ /* On IBM z/OS, pthread_t is a struct with an 8-byte '__' field. The first three bytes of this field appear to uniquely identify a pthread_t, though not necessarily representing a pointer. */ # define gl_thread_self() \ (pthread_in_use () ? pthread_self () : gl_null_thread) # define gl_thread_self_pointer() \ (pthread_in_use () ? *((void **) pthread_self ().__) : NULL) extern const gl_thread_t gl_null_thread; # else # define gl_thread_self() \ (pthread_in_use () ? pthread_self () : (pthread_t) NULL) # define gl_thread_self_pointer() \ (pthread_in_use () ? (void *) pthread_self () : NULL) # endif # define gl_thread_exit(RETVAL) \ (pthread_in_use () ? pthread_exit (RETVAL) : 0) # if HAVE_PTHREAD_ATFORK # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) \ (pthread_in_use () ? pthread_atfork (PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) : 0) # else # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 # endif # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if USE_PTH_THREADS_WEAK /* Use weak references to the GNU Pth threads library. */ # pragma weak pth_init # pragma weak pth_spawn # pragma weak pth_sigmask # pragma weak pth_join # pragma weak pth_self # pragma weak pth_exit # pragma weak pth_cancel # define pth_in_use() (pth_cancel != NULL) # else # define pth_in_use() 1 # endif /* -------------------------- gl_thread_t datatype -------------------------- */ typedef pth_t gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ (pth_in_use () ? (pth_init (), ((*(THREADP) = pth_spawn (NULL, FUNC, ARG)) ? 0 : errno)) : 0) # define glthread_sigmask(HOW, SET, OSET) \ (pth_in_use () ? (pth_init (), (pth_sigmask (HOW, SET, OSET) ? 0 : errno)) : 0) # define glthread_join(THREAD, RETVALP) \ (pth_in_use () ? (pth_init (), (pth_join (THREAD, RETVALP) ? 0 : errno)) : 0) # define gl_thread_self() \ (pth_in_use () ? (pth_init (), (void *) pth_self ()) : NULL) # define gl_thread_self_pointer() \ gl_thread_self () # define gl_thread_exit(RETVAL) \ (pth_in_use () ? (pth_init (), pth_exit (RETVAL)) : 0) # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ # include # include # ifdef __cplusplus extern "C" { # endif # if USE_SOLARIS_THREADS_WEAK /* Use weak references to the old Solaris threads library. */ # pragma weak thr_create # pragma weak thr_join # pragma weak thr_self # pragma weak thr_exit # pragma weak thr_suspend # define thread_in_use() (thr_suspend != NULL) # else # define thread_in_use() 1 # endif /* -------------------------- gl_thread_t datatype -------------------------- */ typedef thread_t gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ (thread_in_use () ? thr_create (NULL, 0, FUNC, ARG, 0, THREADP) : 0) # define glthread_sigmask(HOW, SET, OSET) \ (thread_in_use () ? sigprocmask (HOW, SET, OSET) : 0) # define glthread_join(THREAD, RETVALP) \ (thread_in_use () ? thr_join (THREAD, NULL, RETVALP) : 0) # define gl_thread_self() \ (thread_in_use () ? (void *) thr_self () : NULL) # define gl_thread_self_pointer() \ gl_thread_self () # define gl_thread_exit(RETVAL) \ (thread_in_use () ? thr_exit (RETVAL) : 0) # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # ifdef __cplusplus extern "C" { # endif /* -------------------------- gl_thread_t datatype -------------------------- */ /* The gl_thread_t is a pointer to a structure in memory. Why not the thread handle? If it were the thread handle, it would be hard to implement gl_thread_self() (since GetCurrentThread () returns a pseudo- handle, DuplicateHandle (GetCurrentThread ()) returns a handle that must be closed afterwards, and there is no function for quickly retrieving a thread handle from its id). Why not the thread id? I tried it. It did not work: Sometimes ids appeared that did not belong to running threads, and glthread_join failed with ESRCH. */ typedef struct gl_thread_struct *gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) \ glthread_create_func (THREADP, FUNC, ARG) # define glthread_sigmask(HOW, SET, OSET) \ /* unsupported */ 0 # define glthread_join(THREAD, RETVALP) \ glthread_join_func (THREAD, RETVALP) # define gl_thread_self() \ gl_thread_self_func () # define gl_thread_self_pointer() \ gl_thread_self () # define gl_thread_exit(RETVAL) \ gl_thread_exit_func (RETVAL) # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 extern int glthread_create_func (gl_thread_t *threadp, void * (*func) (void *), void *arg); extern int glthread_join_func (gl_thread_t thread, void **retvalp); extern gl_thread_t gl_thread_self_func (void); extern int gl_thread_exit_func (void *retval); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if !(USE_POSIX_THREADS || USE_PTH_THREADS || USE_SOLARIS_THREADS || USE_WINDOWS_THREADS) /* Provide dummy implementation if threads are not supported. */ typedef int gl_thread_t; # define glthread_create(THREADP, FUNC, ARG) ENOSYS # define glthread_sigmask(HOW, SET, OSET) 0 # define glthread_join(THREAD, RETVALP) 0 # define gl_thread_self() 0 # define gl_thread_self_pointer() \ ((void *) gl_thread_self ()) # define gl_thread_exit(RETVAL) 0 # define glthread_atfork(PREPARE_FUNC, PARENT_FUNC, CHILD_FUNC) 0 #endif /* ========================================================================= */ /* Macros with built-in error handling. */ #ifdef __cplusplus extern "C" { #endif _GLTHREAD_THREAD_INLINE gl_thread_t gl_thread_create (void *(*func) (void *arg), void *arg) { gl_thread_t thread; int ret; ret = glthread_create (&thread, func, arg); if (ret != 0) abort (); return thread; } #define gl_thread_sigmask(HOW, SET, OSET) \ do \ { \ if (glthread_sigmask (HOW, SET, OSET)) \ abort (); \ } \ while (0) #define gl_thread_join(THREAD, RETVAL) \ do \ { \ if (glthread_join (THREAD, RETVAL)) \ abort (); \ } \ while (0) #define gl_thread_atfork(PREPARE, PARENT, CHILD) \ do \ { \ if (glthread_atfork (PREPARE, PARENT, CHILD)) \ abort (); \ } \ while (0) #ifdef __cplusplus } #endif _GL_INLINE_HEADER_END #endif /* _GLTHREAD_THREAD_H */ gnuastro-0.5/bootstrapped/lib/0000755000175000017500000000000013217220465013477 500000000000000gnuastro-0.5/bootstrapped/lib/wctype.in.h0000644000175000017500000003321313217200022015475 00000000000000/* A substitute for ISO C99 , for platforms that lack it. Copyright (C) 2006-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible and Paul Eggert. */ /* * ISO C 99 for platforms that lack it. * * * iswctype, towctrans, towlower, towupper, wctrans, wctype, * wctrans_t, and wctype_t are not yet implemented. */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if (defined __MINGW32__ && defined __CTYPE_H_SOURCED__) /* Special invocation convention: - With MinGW 3.22, when includes , only some part of is being processed, which doesn't include the idempotency guard. */ #@INCLUDE_NEXT@ @NEXT_WCTYPE_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_WCTYPE_H #if @HAVE_WINT_T@ /* Solaris 2.5 has a bug: must be included before . Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ # include # include # include # include #endif /* Native Windows (mingw, MSVC) have declarations of towupper, towlower, and isw* functions in , as well as in . Include , in advance to avoid rpl_ prefix being added to the declarations. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include # include #endif /* Include the original if it exists. BeOS 5 has the functions but no . */ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_WCTYPE_H@ # @INCLUDE_NEXT@ @NEXT_WCTYPE_H@ #endif #ifndef _@GUARD_PREFIX@_WCTYPE_H #define _@GUARD_PREFIX@_WCTYPE_H #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_WCTYPE_INLINE # define _GL_WCTYPE_INLINE _GL_INLINE #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Solaris 2.6 includes which includes which #defines a number of identifiers in the application namespace. Revert these #defines. */ #ifdef __sun # undef multibyte # undef eucw1 # undef eucw2 # undef eucw3 # undef scrw1 # undef scrw2 # undef scrw3 #endif /* Define wint_t and WEOF. (Also done in wchar.in.h.) */ #if !@HAVE_WINT_T@ && !defined wint_t # define wint_t int # ifndef WEOF # define WEOF -1 # endif #else /* mingw and MSVC define wint_t as 'unsigned short' in or . This is too small: ISO C 99 section 7.24.1.(2) says that wint_t must be "unchanged by default argument promotions". Override it. */ # if @GNULIB_OVERRIDES_WINT_T@ # if !GNULIB_defined_wint_t # if @HAVE_CRTDEFS_H@ # include # else # include # endif typedef unsigned int rpl_wint_t; # undef wint_t # define wint_t rpl_wint_t # define GNULIB_defined_wint_t 1 # endif # endif # ifndef WEOF # define WEOF ((wint_t) -1) # endif #endif #if !GNULIB_defined_wctype_functions /* FreeBSD 4.4 to 4.11 has but lacks the functions. Linux libc5 has and the functions but they are broken. Assume all 11 functions (all isw* except iswblank) are implemented the same way, or not at all. */ # if ! @HAVE_ISWCNTRL@ || @REPLACE_ISWCNTRL@ /* IRIX 5.3 has macros but no functions, its isw* macros refer to an undefined variable _ctmp_ and to macros like _P, and they refer to system functions like _iswctype that are not in the standard C library. Rather than try to get ancient buggy implementations like this to work, just disable them. */ # undef iswalnum # undef iswalpha # undef iswblank # undef iswcntrl # undef iswdigit # undef iswgraph # undef iswlower # undef iswprint # undef iswpunct # undef iswspace # undef iswupper # undef iswxdigit # undef towlower # undef towupper /* Linux libc5 has and the functions but they are broken. */ # if @REPLACE_ISWCNTRL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define iswalnum rpl_iswalnum # define iswalpha rpl_iswalpha # define iswblank rpl_iswblank # define iswcntrl rpl_iswcntrl # define iswdigit rpl_iswdigit # define iswgraph rpl_iswgraph # define iswlower rpl_iswlower # define iswprint rpl_iswprint # define iswpunct rpl_iswpunct # define iswspace rpl_iswspace # define iswupper rpl_iswupper # define iswxdigit rpl_iswxdigit # endif # endif # if @REPLACE_TOWLOWER@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define towlower rpl_towlower # define towupper rpl_towupper # endif # endif _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswalnum # else iswalnum # endif (wint_t wc) { return ((wc >= '0' && wc <= '9') || ((wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'Z')); } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswalpha # else iswalpha # endif (wint_t wc) { return (wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'Z'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswblank # else iswblank # endif (wint_t wc) { return wc == ' ' || wc == '\t'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswcntrl # else iswcntrl # endif (wint_t wc) { return (wc & ~0x1f) == 0 || wc == 0x7f; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswdigit # else iswdigit # endif (wint_t wc) { return wc >= '0' && wc <= '9'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswgraph # else iswgraph # endif (wint_t wc) { return wc >= '!' && wc <= '~'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswlower # else iswlower # endif (wint_t wc) { return wc >= 'a' && wc <= 'z'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswprint # else iswprint # endif (wint_t wc) { return wc >= ' ' && wc <= '~'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswpunct # else iswpunct # endif (wint_t wc) { return (wc >= '!' && wc <= '~' && !((wc >= '0' && wc <= '9') || ((wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'Z'))); } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswspace # else iswspace # endif (wint_t wc) { return (wc == ' ' || wc == '\t' || wc == '\n' || wc == '\v' || wc == '\f' || wc == '\r'); } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswupper # else iswupper # endif (wint_t wc) { return wc >= 'A' && wc <= 'Z'; } _GL_WCTYPE_INLINE int # if @REPLACE_ISWCNTRL@ rpl_iswxdigit # else iswxdigit # endif (wint_t wc) { return ((wc >= '0' && wc <= '9') || ((wc & ~0x20) >= 'A' && (wc & ~0x20) <= 'F')); } _GL_WCTYPE_INLINE wint_t # if @REPLACE_TOWLOWER@ rpl_towlower # else towlower # endif (wint_t wc) { return (wc >= 'A' && wc <= 'Z' ? wc - 'A' + 'a' : wc); } _GL_WCTYPE_INLINE wint_t # if @REPLACE_TOWLOWER@ rpl_towupper # else towupper # endif (wint_t wc) { return (wc >= 'a' && wc <= 'z' ? wc - 'a' + 'A' : wc); } # elif @GNULIB_ISWBLANK@ && (! @HAVE_ISWBLANK@ || @REPLACE_ISWBLANK@) /* Only the iswblank function is missing. */ # if @REPLACE_ISWBLANK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define iswblank rpl_iswblank # endif _GL_FUNCDECL_RPL (iswblank, int, (wint_t wc)); # else _GL_FUNCDECL_SYS (iswblank, int, (wint_t wc)); # endif # endif # if defined __MINGW32__ /* On native Windows, wchar_t is uint16_t, and wint_t is uint32_t. The functions towlower and towupper are implemented in the MSVCRT library to take a wchar_t argument and return a wchar_t result. mingw declares these functions to take a wint_t argument and return a wint_t result. This means that: 1. When the user passes an argument outside the range 0x0000..0xFFFF, the function will look only at the lower 16 bits. This is allowed according to POSIX. 2. The return value is returned in the lower 16 bits of the result register. The upper 16 bits are random: whatever happened to be in that part of the result register. We need to fix this by adding a zero-extend from wchar_t to wint_t after the call. */ _GL_WCTYPE_INLINE wint_t rpl_towlower (wint_t wc) { return (wint_t) (wchar_t) towlower (wc); } # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define towlower rpl_towlower # endif _GL_WCTYPE_INLINE wint_t rpl_towupper (wint_t wc) { return (wint_t) (wchar_t) towupper (wc); } # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define towupper rpl_towupper # endif # endif /* __MINGW32__ */ # define GNULIB_defined_wctype_functions 1 #endif #if @REPLACE_ISWCNTRL@ _GL_CXXALIAS_RPL (iswalnum, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswalpha, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswcntrl, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswdigit, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswgraph, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswlower, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswprint, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswpunct, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswspace, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswupper, int, (wint_t wc)); _GL_CXXALIAS_RPL (iswxdigit, int, (wint_t wc)); #else _GL_CXXALIAS_SYS (iswalnum, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswalpha, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswcntrl, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswdigit, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswgraph, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswlower, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswprint, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswpunct, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswspace, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswupper, int, (wint_t wc)); _GL_CXXALIAS_SYS (iswxdigit, int, (wint_t wc)); #endif _GL_CXXALIASWARN (iswalnum); _GL_CXXALIASWARN (iswalpha); _GL_CXXALIASWARN (iswcntrl); _GL_CXXALIASWARN (iswdigit); _GL_CXXALIASWARN (iswgraph); _GL_CXXALIASWARN (iswlower); _GL_CXXALIASWARN (iswprint); _GL_CXXALIASWARN (iswpunct); _GL_CXXALIASWARN (iswspace); _GL_CXXALIASWARN (iswupper); _GL_CXXALIASWARN (iswxdigit); #if @GNULIB_ISWBLANK@ # if @REPLACE_ISWCNTRL@ || @REPLACE_ISWBLANK@ _GL_CXXALIAS_RPL (iswblank, int, (wint_t wc)); # else _GL_CXXALIAS_SYS (iswblank, int, (wint_t wc)); # endif _GL_CXXALIASWARN (iswblank); #endif #if !@HAVE_WCTYPE_T@ # if !GNULIB_defined_wctype_t typedef void * wctype_t; # define GNULIB_defined_wctype_t 1 # endif #endif /* Get a descriptor for a wide character property. */ #if @GNULIB_WCTYPE@ # if !@HAVE_WCTYPE_T@ _GL_FUNCDECL_SYS (wctype, wctype_t, (const char *name)); # endif _GL_CXXALIAS_SYS (wctype, wctype_t, (const char *name)); _GL_CXXALIASWARN (wctype); #elif defined GNULIB_POSIXCHECK # undef wctype # if HAVE_RAW_DECL_WCTYPE _GL_WARN_ON_USE (wctype, "wctype is unportable - " "use gnulib module wctype for portability"); # endif #endif /* Test whether a wide character has a given property. The argument WC must be either a wchar_t value or WEOF. The argument DESC must have been returned by the wctype() function. */ #if @GNULIB_ISWCTYPE@ # if !@HAVE_WCTYPE_T@ _GL_FUNCDECL_SYS (iswctype, int, (wint_t wc, wctype_t desc)); # endif _GL_CXXALIAS_SYS (iswctype, int, (wint_t wc, wctype_t desc)); _GL_CXXALIASWARN (iswctype); #elif defined GNULIB_POSIXCHECK # undef iswctype # if HAVE_RAW_DECL_ISWCTYPE _GL_WARN_ON_USE (iswctype, "iswctype is unportable - " "use gnulib module iswctype for portability"); # endif #endif #if @REPLACE_TOWLOWER@ || defined __MINGW32__ _GL_CXXALIAS_RPL (towlower, wint_t, (wint_t wc)); _GL_CXXALIAS_RPL (towupper, wint_t, (wint_t wc)); #else _GL_CXXALIAS_SYS (towlower, wint_t, (wint_t wc)); _GL_CXXALIAS_SYS (towupper, wint_t, (wint_t wc)); #endif _GL_CXXALIASWARN (towlower); _GL_CXXALIASWARN (towupper); #if !@HAVE_WCTRANS_T@ # if !GNULIB_defined_wctrans_t typedef void * wctrans_t; # define GNULIB_defined_wctrans_t 1 # endif #endif /* Get a descriptor for a wide character case conversion. */ #if @GNULIB_WCTRANS@ # if !@HAVE_WCTRANS_T@ _GL_FUNCDECL_SYS (wctrans, wctrans_t, (const char *name)); # endif _GL_CXXALIAS_SYS (wctrans, wctrans_t, (const char *name)); _GL_CXXALIASWARN (wctrans); #elif defined GNULIB_POSIXCHECK # undef wctrans # if HAVE_RAW_DECL_WCTRANS _GL_WARN_ON_USE (wctrans, "wctrans is unportable - " "use gnulib module wctrans for portability"); # endif #endif /* Perform a given case conversion on a wide character. The argument WC must be either a wchar_t value or WEOF. The argument DESC must have been returned by the wctrans() function. */ #if @GNULIB_TOWCTRANS@ # if !@HAVE_WCTRANS_T@ _GL_FUNCDECL_SYS (towctrans, wint_t, (wint_t wc, wctrans_t desc)); # endif _GL_CXXALIAS_SYS (towctrans, wint_t, (wint_t wc, wctrans_t desc)); _GL_CXXALIASWARN (towctrans); #elif defined GNULIB_POSIXCHECK # undef towctrans # if HAVE_RAW_DECL_TOWCTRANS _GL_WARN_ON_USE (towctrans, "towctrans is unportable - " "use gnulib module towctrans for portability"); # endif #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_WCTYPE_H */ #endif /* _@GUARD_PREFIX@_WCTYPE_H */ #endif gnuastro-0.5/bootstrapped/lib/wchar.in.h0000644000175000017500000010542613217200022015274 00000000000000/* A substitute for ISO C99 , for platforms that have issues. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake. */ /* * ISO C 99 for platforms that have issues. * * * For now, this just ensures proper prerequisite inclusion order and * the declaration of wcwidth(). */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if (((defined __need_mbstate_t || defined __need_wint_t) \ && !defined __MINGW32__) \ || (defined __hpux \ && ((defined _INTTYPES_INCLUDED && !defined strtoimax) \ || defined _GL_JUST_INCLUDE_SYSTEM_WCHAR_H)) \ || (defined __MINGW32__ && defined __STRING_H_SOURCED__) \ || defined _GL_ALREADY_INCLUDING_WCHAR_H) /* Special invocation convention: - Inside glibc and uClibc header files, but not MinGW. - On HP-UX 11.00 we have a sequence of nested includes -> -> , and the latter includes , once indirectly -> -> -> and once directly. In both situations 'wint_t' is not yet defined, therefore we cannot provide the function overrides; instead include only the system's . - With MinGW 3.22, when includes , only some part of is actually processed, and that doesn't include 'mbstate_t'. - On IRIX 6.5, similarly, we have an include -> , and the latter includes . But here, we have no way to detect whether is completely included or is still being included. */ #@INCLUDE_NEXT@ @NEXT_WCHAR_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_WCHAR_H #define _GL_ALREADY_INCLUDING_WCHAR_H #if @HAVE_FEATURES_H@ # include /* for __GLIBC__ */ #endif /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . In some builds of uClibc, is nonexistent and wchar_t is defined by . But avoid namespace pollution on glibc systems. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include #endif #ifndef __GLIBC__ # include # include #endif /* Include the original if it exists. Some builds of uClibc lack it. */ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_WCHAR_H@ # @INCLUDE_NEXT@ @NEXT_WCHAR_H@ #endif #undef _GL_ALREADY_INCLUDING_WCHAR_H #ifndef _@GUARD_PREFIX@_WCHAR_H #define _@GUARD_PREFIX@_WCHAR_H /* The __attribute__ feature is available in gcc versions 2.5 and later. The attribute __pure__ was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Define wint_t and WEOF. (Also done in wctype.in.h.) */ #if !@HAVE_WINT_T@ && !defined wint_t # define wint_t int # ifndef WEOF # define WEOF -1 # endif #else /* mingw and MSVC define wint_t as 'unsigned short' in or . This is too small: ISO C 99 section 7.24.1.(2) says that wint_t must be "unchanged by default argument promotions". Override it. */ # if @GNULIB_OVERRIDES_WINT_T@ # if !GNULIB_defined_wint_t # if @HAVE_CRTDEFS_H@ # include # else # include # endif typedef unsigned int rpl_wint_t; # undef wint_t # define wint_t rpl_wint_t # define GNULIB_defined_wint_t 1 # endif # endif # ifndef WEOF # define WEOF ((wint_t) -1) # endif #endif /* Override mbstate_t if it is too small. On IRIX 6.5, sizeof (mbstate_t) == 1, which is not sufficient for implementing mbrtowc for encodings like UTF-8. */ #if !(@HAVE_MBSINIT@ && @HAVE_MBRTOWC@) || @REPLACE_MBSTATE_T@ # if !GNULIB_defined_mbstate_t typedef int rpl_mbstate_t; # undef mbstate_t # define mbstate_t rpl_mbstate_t # define GNULIB_defined_mbstate_t 1 # endif #endif /* Convert a single-byte character to a wide character. */ #if @GNULIB_BTOWC@ # if @REPLACE_BTOWC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef btowc # define btowc rpl_btowc # endif _GL_FUNCDECL_RPL (btowc, wint_t, (int c) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (btowc, wint_t, (int c)); # else # if !@HAVE_BTOWC@ _GL_FUNCDECL_SYS (btowc, wint_t, (int c) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (btowc, wint_t, (int c)); # endif _GL_CXXALIASWARN (btowc); #elif defined GNULIB_POSIXCHECK # undef btowc # if HAVE_RAW_DECL_BTOWC _GL_WARN_ON_USE (btowc, "btowc is unportable - " "use gnulib module btowc for portability"); # endif #endif /* Convert a wide character to a single-byte character. */ #if @GNULIB_WCTOB@ # if @REPLACE_WCTOB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wctob # define wctob rpl_wctob # endif _GL_FUNCDECL_RPL (wctob, int, (wint_t wc) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (wctob, int, (wint_t wc)); # else # if !defined wctob && !@HAVE_DECL_WCTOB@ /* wctob is provided by gnulib, or wctob exists but is not declared. */ _GL_FUNCDECL_SYS (wctob, int, (wint_t wc) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wctob, int, (wint_t wc)); # endif _GL_CXXALIASWARN (wctob); #elif defined GNULIB_POSIXCHECK # undef wctob # if HAVE_RAW_DECL_WCTOB _GL_WARN_ON_USE (wctob, "wctob is unportable - " "use gnulib module wctob for portability"); # endif #endif /* Test whether *PS is in the initial state. */ #if @GNULIB_MBSINIT@ # if @REPLACE_MBSINIT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbsinit # define mbsinit rpl_mbsinit # endif _GL_FUNCDECL_RPL (mbsinit, int, (const mbstate_t *ps)); _GL_CXXALIAS_RPL (mbsinit, int, (const mbstate_t *ps)); # else # if !@HAVE_MBSINIT@ _GL_FUNCDECL_SYS (mbsinit, int, (const mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (mbsinit, int, (const mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbsinit); #elif defined GNULIB_POSIXCHECK # undef mbsinit # if HAVE_RAW_DECL_MBSINIT _GL_WARN_ON_USE (mbsinit, "mbsinit is unportable - " "use gnulib module mbsinit for portability"); # endif #endif /* Convert a multibyte character to a wide character. */ #if @GNULIB_MBRTOWC@ # if @REPLACE_MBRTOWC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbrtowc # define mbrtowc rpl_mbrtowc # endif _GL_FUNCDECL_RPL (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); _GL_CXXALIAS_RPL (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); # else # if !@HAVE_MBRTOWC@ _GL_FUNCDECL_SYS (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (mbrtowc, size_t, (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbrtowc); #elif defined GNULIB_POSIXCHECK # undef mbrtowc # if HAVE_RAW_DECL_MBRTOWC _GL_WARN_ON_USE (mbrtowc, "mbrtowc is unportable - " "use gnulib module mbrtowc for portability"); # endif #endif /* Recognize a multibyte character. */ #if @GNULIB_MBRLEN@ # if @REPLACE_MBRLEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbrlen # define mbrlen rpl_mbrlen # endif _GL_FUNCDECL_RPL (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); _GL_CXXALIAS_RPL (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); # else # if !@HAVE_MBRLEN@ _GL_FUNCDECL_SYS (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (mbrlen, size_t, (const char *s, size_t n, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbrlen); #elif defined GNULIB_POSIXCHECK # undef mbrlen # if HAVE_RAW_DECL_MBRLEN _GL_WARN_ON_USE (mbrlen, "mbrlen is unportable - " "use gnulib module mbrlen for portability"); # endif #endif /* Convert a string to a wide string. */ #if @GNULIB_MBSRTOWCS@ # if @REPLACE_MBSRTOWCS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbsrtowcs # define mbsrtowcs rpl_mbsrtowcs # endif _GL_FUNCDECL_RPL (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps)); # else # if !@HAVE_MBSRTOWCS@ _GL_FUNCDECL_SYS (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mbsrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbsrtowcs); #elif defined GNULIB_POSIXCHECK # undef mbsrtowcs # if HAVE_RAW_DECL_MBSRTOWCS _GL_WARN_ON_USE (mbsrtowcs, "mbsrtowcs is unportable - " "use gnulib module mbsrtowcs for portability"); # endif #endif /* Convert a string to a wide string. */ #if @GNULIB_MBSNRTOWCS@ # if @REPLACE_MBSNRTOWCS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbsnrtowcs # define mbsnrtowcs rpl_mbsnrtowcs # endif _GL_FUNCDECL_RPL (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps)); # else # if !@HAVE_MBSNRTOWCS@ _GL_FUNCDECL_SYS (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (mbsnrtowcs, size_t, (wchar_t *dest, const char **srcp, size_t srclen, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (mbsnrtowcs); #elif defined GNULIB_POSIXCHECK # undef mbsnrtowcs # if HAVE_RAW_DECL_MBSNRTOWCS _GL_WARN_ON_USE (mbsnrtowcs, "mbsnrtowcs is unportable - " "use gnulib module mbsnrtowcs for portability"); # endif #endif /* Convert a wide character to a multibyte character. */ #if @GNULIB_WCRTOMB@ # if @REPLACE_WCRTOMB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcrtomb # define wcrtomb rpl_wcrtomb # endif _GL_FUNCDECL_RPL (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); _GL_CXXALIAS_RPL (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); # else # if !@HAVE_WCRTOMB@ _GL_FUNCDECL_SYS (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); # endif _GL_CXXALIAS_SYS (wcrtomb, size_t, (char *s, wchar_t wc, mbstate_t *ps)); # endif _GL_CXXALIASWARN (wcrtomb); #elif defined GNULIB_POSIXCHECK # undef wcrtomb # if HAVE_RAW_DECL_WCRTOMB _GL_WARN_ON_USE (wcrtomb, "wcrtomb is unportable - " "use gnulib module wcrtomb for portability"); # endif #endif /* Convert a wide string to a string. */ #if @GNULIB_WCSRTOMBS@ # if @REPLACE_WCSRTOMBS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcsrtombs # define wcsrtombs rpl_wcsrtombs # endif _GL_FUNCDECL_RPL (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps)); # else # if !@HAVE_WCSRTOMBS@ _GL_FUNCDECL_SYS (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (wcsrtombs, size_t, (char *dest, const wchar_t **srcp, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (wcsrtombs); #elif defined GNULIB_POSIXCHECK # undef wcsrtombs # if HAVE_RAW_DECL_WCSRTOMBS _GL_WARN_ON_USE (wcsrtombs, "wcsrtombs is unportable - " "use gnulib module wcsrtombs for portability"); # endif #endif /* Convert a wide string to a string. */ #if @GNULIB_WCSNRTOMBS@ # if @REPLACE_WCSNRTOMBS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcsnrtombs # define wcsnrtombs rpl_wcsnrtombs # endif _GL_FUNCDECL_RPL (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps)); # else # if !@HAVE_WCSNRTOMBS@ _GL_FUNCDECL_SYS (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (wcsnrtombs, size_t, (char *dest, const wchar_t **srcp, size_t srclen, size_t len, mbstate_t *ps)); # endif _GL_CXXALIASWARN (wcsnrtombs); #elif defined GNULIB_POSIXCHECK # undef wcsnrtombs # if HAVE_RAW_DECL_WCSNRTOMBS _GL_WARN_ON_USE (wcsnrtombs, "wcsnrtombs is unportable - " "use gnulib module wcsnrtombs for portability"); # endif #endif /* Return the number of screen columns needed for WC. */ #if @GNULIB_WCWIDTH@ # if @REPLACE_WCWIDTH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcwidth # define wcwidth rpl_wcwidth # endif _GL_FUNCDECL_RPL (wcwidth, int, (wchar_t) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (wcwidth, int, (wchar_t)); # else # if !@HAVE_DECL_WCWIDTH@ /* wcwidth exists but is not declared. */ _GL_FUNCDECL_SYS (wcwidth, int, (wchar_t) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcwidth, int, (wchar_t)); # endif _GL_CXXALIASWARN (wcwidth); #elif defined GNULIB_POSIXCHECK # undef wcwidth # if HAVE_RAW_DECL_WCWIDTH _GL_WARN_ON_USE (wcwidth, "wcwidth is unportable - " "use gnulib module wcwidth for portability"); # endif #endif /* Search N wide characters of S for C. */ #if @GNULIB_WMEMCHR@ # if !@HAVE_WMEMCHR@ _GL_FUNCDECL_SYS (wmemchr, wchar_t *, (const wchar_t *s, wchar_t c, size_t n) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wmemchr (const wchar_t *, wchar_t, size_t); wchar_t * std::wmemchr (wchar_t *, wchar_t, size_t); } */ _GL_CXXALIAS_SYS_CAST2 (wmemchr, wchar_t *, (const wchar_t *, wchar_t, size_t), const wchar_t *, (const wchar_t *, wchar_t, size_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wmemchr, wchar_t *, (wchar_t *s, wchar_t c, size_t n)); _GL_CXXALIASWARN1 (wmemchr, const wchar_t *, (const wchar_t *s, wchar_t c, size_t n)); # else _GL_CXXALIASWARN (wmemchr); # endif #elif defined GNULIB_POSIXCHECK # undef wmemchr # if HAVE_RAW_DECL_WMEMCHR _GL_WARN_ON_USE (wmemchr, "wmemchr is unportable - " "use gnulib module wmemchr for portability"); # endif #endif /* Compare N wide characters of S1 and S2. */ #if @GNULIB_WMEMCMP@ # if !@HAVE_WMEMCMP@ _GL_FUNCDECL_SYS (wmemcmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wmemcmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wmemcmp); #elif defined GNULIB_POSIXCHECK # undef wmemcmp # if HAVE_RAW_DECL_WMEMCMP _GL_WARN_ON_USE (wmemcmp, "wmemcmp is unportable - " "use gnulib module wmemcmp for portability"); # endif #endif /* Copy N wide characters of SRC to DEST. */ #if @GNULIB_WMEMCPY@ # if !@HAVE_WMEMCPY@ _GL_FUNCDECL_SYS (wmemcpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wmemcpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wmemcpy); #elif defined GNULIB_POSIXCHECK # undef wmemcpy # if HAVE_RAW_DECL_WMEMCPY _GL_WARN_ON_USE (wmemcpy, "wmemcpy is unportable - " "use gnulib module wmemcpy for portability"); # endif #endif /* Copy N wide characters of SRC to DEST, guaranteeing correct behavior for overlapping memory areas. */ #if @GNULIB_WMEMMOVE@ # if !@HAVE_WMEMMOVE@ _GL_FUNCDECL_SYS (wmemmove, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wmemmove, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wmemmove); #elif defined GNULIB_POSIXCHECK # undef wmemmove # if HAVE_RAW_DECL_WMEMMOVE _GL_WARN_ON_USE (wmemmove, "wmemmove is unportable - " "use gnulib module wmemmove for portability"); # endif #endif /* Set N wide characters of S to C. */ #if @GNULIB_WMEMSET@ # if !@HAVE_WMEMSET@ _GL_FUNCDECL_SYS (wmemset, wchar_t *, (wchar_t *s, wchar_t c, size_t n)); # endif _GL_CXXALIAS_SYS (wmemset, wchar_t *, (wchar_t *s, wchar_t c, size_t n)); _GL_CXXALIASWARN (wmemset); #elif defined GNULIB_POSIXCHECK # undef wmemset # if HAVE_RAW_DECL_WMEMSET _GL_WARN_ON_USE (wmemset, "wmemset is unportable - " "use gnulib module wmemset for portability"); # endif #endif /* Return the number of wide characters in S. */ #if @GNULIB_WCSLEN@ # if !@HAVE_WCSLEN@ _GL_FUNCDECL_SYS (wcslen, size_t, (const wchar_t *s) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcslen, size_t, (const wchar_t *s)); _GL_CXXALIASWARN (wcslen); #elif defined GNULIB_POSIXCHECK # undef wcslen # if HAVE_RAW_DECL_WCSLEN _GL_WARN_ON_USE (wcslen, "wcslen is unportable - " "use gnulib module wcslen for portability"); # endif #endif /* Return the number of wide characters in S, but at most MAXLEN. */ #if @GNULIB_WCSNLEN@ # if !@HAVE_WCSNLEN@ _GL_FUNCDECL_SYS (wcsnlen, size_t, (const wchar_t *s, size_t maxlen) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsnlen, size_t, (const wchar_t *s, size_t maxlen)); _GL_CXXALIASWARN (wcsnlen); #elif defined GNULIB_POSIXCHECK # undef wcsnlen # if HAVE_RAW_DECL_WCSNLEN _GL_WARN_ON_USE (wcsnlen, "wcsnlen is unportable - " "use gnulib module wcsnlen for portability"); # endif #endif /* Copy SRC to DEST. */ #if @GNULIB_WCSCPY@ # if !@HAVE_WCSCPY@ _GL_FUNCDECL_SYS (wcscpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); # endif _GL_CXXALIAS_SYS (wcscpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); _GL_CXXALIASWARN (wcscpy); #elif defined GNULIB_POSIXCHECK # undef wcscpy # if HAVE_RAW_DECL_WCSCPY _GL_WARN_ON_USE (wcscpy, "wcscpy is unportable - " "use gnulib module wcscpy for portability"); # endif #endif /* Copy SRC to DEST, returning the address of the terminating L'\0' in DEST. */ #if @GNULIB_WCPCPY@ # if !@HAVE_WCPCPY@ _GL_FUNCDECL_SYS (wcpcpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); # endif _GL_CXXALIAS_SYS (wcpcpy, wchar_t *, (wchar_t *dest, const wchar_t *src)); _GL_CXXALIASWARN (wcpcpy); #elif defined GNULIB_POSIXCHECK # undef wcpcpy # if HAVE_RAW_DECL_WCPCPY _GL_WARN_ON_USE (wcpcpy, "wcpcpy is unportable - " "use gnulib module wcpcpy for portability"); # endif #endif /* Copy no more than N wide characters of SRC to DEST. */ #if @GNULIB_WCSNCPY@ # if !@HAVE_WCSNCPY@ _GL_FUNCDECL_SYS (wcsncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wcsncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wcsncpy); #elif defined GNULIB_POSIXCHECK # undef wcsncpy # if HAVE_RAW_DECL_WCSNCPY _GL_WARN_ON_USE (wcsncpy, "wcsncpy is unportable - " "use gnulib module wcsncpy for portability"); # endif #endif /* Copy no more than N characters of SRC to DEST, returning the address of the last character written into DEST. */ #if @GNULIB_WCPNCPY@ # if !@HAVE_WCPNCPY@ _GL_FUNCDECL_SYS (wcpncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wcpncpy, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wcpncpy); #elif defined GNULIB_POSIXCHECK # undef wcpncpy # if HAVE_RAW_DECL_WCPNCPY _GL_WARN_ON_USE (wcpncpy, "wcpncpy is unportable - " "use gnulib module wcpncpy for portability"); # endif #endif /* Append SRC onto DEST. */ #if @GNULIB_WCSCAT@ # if !@HAVE_WCSCAT@ _GL_FUNCDECL_SYS (wcscat, wchar_t *, (wchar_t *dest, const wchar_t *src)); # endif _GL_CXXALIAS_SYS (wcscat, wchar_t *, (wchar_t *dest, const wchar_t *src)); _GL_CXXALIASWARN (wcscat); #elif defined GNULIB_POSIXCHECK # undef wcscat # if HAVE_RAW_DECL_WCSCAT _GL_WARN_ON_USE (wcscat, "wcscat is unportable - " "use gnulib module wcscat for portability"); # endif #endif /* Append no more than N wide characters of SRC onto DEST. */ #if @GNULIB_WCSNCAT@ # if !@HAVE_WCSNCAT@ _GL_FUNCDECL_SYS (wcsncat, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); # endif _GL_CXXALIAS_SYS (wcsncat, wchar_t *, (wchar_t *dest, const wchar_t *src, size_t n)); _GL_CXXALIASWARN (wcsncat); #elif defined GNULIB_POSIXCHECK # undef wcsncat # if HAVE_RAW_DECL_WCSNCAT _GL_WARN_ON_USE (wcsncat, "wcsncat is unportable - " "use gnulib module wcsncat for portability"); # endif #endif /* Compare S1 and S2. */ #if @GNULIB_WCSCMP@ # if !@HAVE_WCSCMP@ _GL_FUNCDECL_SYS (wcscmp, int, (const wchar_t *s1, const wchar_t *s2) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcscmp, int, (const wchar_t *s1, const wchar_t *s2)); _GL_CXXALIASWARN (wcscmp); #elif defined GNULIB_POSIXCHECK # undef wcscmp # if HAVE_RAW_DECL_WCSCMP _GL_WARN_ON_USE (wcscmp, "wcscmp is unportable - " "use gnulib module wcscmp for portability"); # endif #endif /* Compare no more than N wide characters of S1 and S2. */ #if @GNULIB_WCSNCMP@ # if !@HAVE_WCSNCMP@ _GL_FUNCDECL_SYS (wcsncmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsncmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wcsncmp); #elif defined GNULIB_POSIXCHECK # undef wcsncmp # if HAVE_RAW_DECL_WCSNCMP _GL_WARN_ON_USE (wcsncmp, "wcsncmp is unportable - " "use gnulib module wcsncmp for portability"); # endif #endif /* Compare S1 and S2, ignoring case. */ #if @GNULIB_WCSCASECMP@ # if !@HAVE_WCSCASECMP@ _GL_FUNCDECL_SYS (wcscasecmp, int, (const wchar_t *s1, const wchar_t *s2) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcscasecmp, int, (const wchar_t *s1, const wchar_t *s2)); _GL_CXXALIASWARN (wcscasecmp); #elif defined GNULIB_POSIXCHECK # undef wcscasecmp # if HAVE_RAW_DECL_WCSCASECMP _GL_WARN_ON_USE (wcscasecmp, "wcscasecmp is unportable - " "use gnulib module wcscasecmp for portability"); # endif #endif /* Compare no more than N chars of S1 and S2, ignoring case. */ #if @GNULIB_WCSNCASECMP@ # if !@HAVE_WCSNCASECMP@ _GL_FUNCDECL_SYS (wcsncasecmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsncasecmp, int, (const wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wcsncasecmp); #elif defined GNULIB_POSIXCHECK # undef wcsncasecmp # if HAVE_RAW_DECL_WCSNCASECMP _GL_WARN_ON_USE (wcsncasecmp, "wcsncasecmp is unportable - " "use gnulib module wcsncasecmp for portability"); # endif #endif /* Compare S1 and S2, both interpreted as appropriate to the LC_COLLATE category of the current locale. */ #if @GNULIB_WCSCOLL@ # if !@HAVE_WCSCOLL@ _GL_FUNCDECL_SYS (wcscoll, int, (const wchar_t *s1, const wchar_t *s2)); # endif _GL_CXXALIAS_SYS (wcscoll, int, (const wchar_t *s1, const wchar_t *s2)); _GL_CXXALIASWARN (wcscoll); #elif defined GNULIB_POSIXCHECK # undef wcscoll # if HAVE_RAW_DECL_WCSCOLL _GL_WARN_ON_USE (wcscoll, "wcscoll is unportable - " "use gnulib module wcscoll for portability"); # endif #endif /* Transform S2 into array pointed to by S1 such that if wcscmp is applied to two transformed strings the result is the as applying 'wcscoll' to the original strings. */ #if @GNULIB_WCSXFRM@ # if !@HAVE_WCSXFRM@ _GL_FUNCDECL_SYS (wcsxfrm, size_t, (wchar_t *s1, const wchar_t *s2, size_t n)); # endif _GL_CXXALIAS_SYS (wcsxfrm, size_t, (wchar_t *s1, const wchar_t *s2, size_t n)); _GL_CXXALIASWARN (wcsxfrm); #elif defined GNULIB_POSIXCHECK # undef wcsxfrm # if HAVE_RAW_DECL_WCSXFRM _GL_WARN_ON_USE (wcsxfrm, "wcsxfrm is unportable - " "use gnulib module wcsxfrm for portability"); # endif #endif /* Duplicate S, returning an identical malloc'd string. */ #if @GNULIB_WCSDUP@ # if !@HAVE_WCSDUP@ _GL_FUNCDECL_SYS (wcsdup, wchar_t *, (const wchar_t *s)); # endif _GL_CXXALIAS_SYS (wcsdup, wchar_t *, (const wchar_t *s)); _GL_CXXALIASWARN (wcsdup); #elif defined GNULIB_POSIXCHECK # undef wcsdup # if HAVE_RAW_DECL_WCSDUP _GL_WARN_ON_USE (wcsdup, "wcsdup is unportable - " "use gnulib module wcsdup for portability"); # endif #endif /* Find the first occurrence of WC in WCS. */ #if @GNULIB_WCSCHR@ # if !@HAVE_WCSCHR@ _GL_FUNCDECL_SYS (wcschr, wchar_t *, (const wchar_t *wcs, wchar_t wc) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcschr (const wchar_t *, wchar_t); wchar_t * std::wcschr (wchar_t *, wchar_t); } */ _GL_CXXALIAS_SYS_CAST2 (wcschr, wchar_t *, (const wchar_t *, wchar_t), const wchar_t *, (const wchar_t *, wchar_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcschr, wchar_t *, (wchar_t *wcs, wchar_t wc)); _GL_CXXALIASWARN1 (wcschr, const wchar_t *, (const wchar_t *wcs, wchar_t wc)); # else _GL_CXXALIASWARN (wcschr); # endif #elif defined GNULIB_POSIXCHECK # undef wcschr # if HAVE_RAW_DECL_WCSCHR _GL_WARN_ON_USE (wcschr, "wcschr is unportable - " "use gnulib module wcschr for portability"); # endif #endif /* Find the last occurrence of WC in WCS. */ #if @GNULIB_WCSRCHR@ # if !@HAVE_WCSRCHR@ _GL_FUNCDECL_SYS (wcsrchr, wchar_t *, (const wchar_t *wcs, wchar_t wc) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcsrchr (const wchar_t *, wchar_t); wchar_t * std::wcsrchr (wchar_t *, wchar_t); } */ _GL_CXXALIAS_SYS_CAST2 (wcsrchr, wchar_t *, (const wchar_t *, wchar_t), const wchar_t *, (const wchar_t *, wchar_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcsrchr, wchar_t *, (wchar_t *wcs, wchar_t wc)); _GL_CXXALIASWARN1 (wcsrchr, const wchar_t *, (const wchar_t *wcs, wchar_t wc)); # else _GL_CXXALIASWARN (wcsrchr); # endif #elif defined GNULIB_POSIXCHECK # undef wcsrchr # if HAVE_RAW_DECL_WCSRCHR _GL_WARN_ON_USE (wcsrchr, "wcsrchr is unportable - " "use gnulib module wcsrchr for portability"); # endif #endif /* Return the length of the initial segmet of WCS which consists entirely of wide characters not in REJECT. */ #if @GNULIB_WCSCSPN@ # if !@HAVE_WCSCSPN@ _GL_FUNCDECL_SYS (wcscspn, size_t, (const wchar_t *wcs, const wchar_t *reject) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcscspn, size_t, (const wchar_t *wcs, const wchar_t *reject)); _GL_CXXALIASWARN (wcscspn); #elif defined GNULIB_POSIXCHECK # undef wcscspn # if HAVE_RAW_DECL_WCSCSPN _GL_WARN_ON_USE (wcscspn, "wcscspn is unportable - " "use gnulib module wcscspn for portability"); # endif #endif /* Return the length of the initial segmet of WCS which consists entirely of wide characters in ACCEPT. */ #if @GNULIB_WCSSPN@ # if !@HAVE_WCSSPN@ _GL_FUNCDECL_SYS (wcsspn, size_t, (const wchar_t *wcs, const wchar_t *accept) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcsspn, size_t, (const wchar_t *wcs, const wchar_t *accept)); _GL_CXXALIASWARN (wcsspn); #elif defined GNULIB_POSIXCHECK # undef wcsspn # if HAVE_RAW_DECL_WCSSPN _GL_WARN_ON_USE (wcsspn, "wcsspn is unportable - " "use gnulib module wcsspn for portability"); # endif #endif /* Find the first occurrence in WCS of any character in ACCEPT. */ #if @GNULIB_WCSPBRK@ # if !@HAVE_WCSPBRK@ _GL_FUNCDECL_SYS (wcspbrk, wchar_t *, (const wchar_t *wcs, const wchar_t *accept) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcspbrk (const wchar_t *, const wchar_t *); wchar_t * std::wcspbrk (wchar_t *, const wchar_t *); } */ _GL_CXXALIAS_SYS_CAST2 (wcspbrk, wchar_t *, (const wchar_t *, const wchar_t *), const wchar_t *, (const wchar_t *, const wchar_t *)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcspbrk, wchar_t *, (wchar_t *wcs, const wchar_t *accept)); _GL_CXXALIASWARN1 (wcspbrk, const wchar_t *, (const wchar_t *wcs, const wchar_t *accept)); # else _GL_CXXALIASWARN (wcspbrk); # endif #elif defined GNULIB_POSIXCHECK # undef wcspbrk # if HAVE_RAW_DECL_WCSPBRK _GL_WARN_ON_USE (wcspbrk, "wcspbrk is unportable - " "use gnulib module wcspbrk for portability"); # endif #endif /* Find the first occurrence of NEEDLE in HAYSTACK. */ #if @GNULIB_WCSSTR@ # if !@HAVE_WCSSTR@ _GL_FUNCDECL_SYS (wcsstr, wchar_t *, (const wchar_t *haystack, const wchar_t *needle) _GL_ATTRIBUTE_PURE); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const wchar_t * std::wcsstr (const wchar_t *, const wchar_t *); wchar_t * std::wcsstr (wchar_t *, const wchar_t *); } */ _GL_CXXALIAS_SYS_CAST2 (wcsstr, wchar_t *, (const wchar_t *, const wchar_t *), const wchar_t *, (const wchar_t *, const wchar_t *)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (wcsstr, wchar_t *, (wchar_t *haystack, const wchar_t *needle)); _GL_CXXALIASWARN1 (wcsstr, const wchar_t *, (const wchar_t *haystack, const wchar_t *needle)); # else _GL_CXXALIASWARN (wcsstr); # endif #elif defined GNULIB_POSIXCHECK # undef wcsstr # if HAVE_RAW_DECL_WCSSTR _GL_WARN_ON_USE (wcsstr, "wcsstr is unportable - " "use gnulib module wcsstr for portability"); # endif #endif /* Divide WCS into tokens separated by characters in DELIM. */ #if @GNULIB_WCSTOK@ # if !@HAVE_WCSTOK@ _GL_FUNCDECL_SYS (wcstok, wchar_t *, (wchar_t *wcs, const wchar_t *delim, wchar_t **ptr)); # endif _GL_CXXALIAS_SYS (wcstok, wchar_t *, (wchar_t *wcs, const wchar_t *delim, wchar_t **ptr)); _GL_CXXALIASWARN (wcstok); #elif defined GNULIB_POSIXCHECK # undef wcstok # if HAVE_RAW_DECL_WCSTOK _GL_WARN_ON_USE (wcstok, "wcstok is unportable - " "use gnulib module wcstok for portability"); # endif #endif /* Determine number of column positions required for first N wide characters (or fewer if S ends before this) in S. */ #if @GNULIB_WCSWIDTH@ # if @REPLACE_WCSWIDTH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcswidth # define wcswidth rpl_wcswidth # endif _GL_FUNCDECL_RPL (wcswidth, int, (const wchar_t *s, size_t n) _GL_ATTRIBUTE_PURE); _GL_CXXALIAS_RPL (wcswidth, int, (const wchar_t *s, size_t n)); # else # if !@HAVE_WCSWIDTH@ _GL_FUNCDECL_SYS (wcswidth, int, (const wchar_t *s, size_t n) _GL_ATTRIBUTE_PURE); # endif _GL_CXXALIAS_SYS (wcswidth, int, (const wchar_t *s, size_t n)); # endif _GL_CXXALIASWARN (wcswidth); #elif defined GNULIB_POSIXCHECK # undef wcswidth # if HAVE_RAW_DECL_WCSWIDTH _GL_WARN_ON_USE (wcswidth, "wcswidth is unportable - " "use gnulib module wcswidth for portability"); # endif #endif /* Convert *TP to a date and time wide string. See . */ #if @GNULIB_WCSFTIME@ # if @REPLACE_WCSFTIME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wcsftime # define wcsftime rpl_wcsftime # endif _GL_FUNCDECL_RPL (wcsftime, size_t, (wchar_t *__buf, size_t __bufsize, const wchar_t *__fmt, const struct tm *__tp) _GL_ARG_NONNULL ((1, 3, 4))); _GL_CXXALIAS_RPL (wcsftime, size_t, (wchar_t *__buf, size_t __bufsize, const wchar_t *__fmt, const struct tm *__tp)); # else # if !@HAVE_WCSFTIME@ _GL_FUNCDECL_SYS (wcsftime, size_t, (wchar_t *__buf, size_t __bufsize, const wchar_t *__fmt, const struct tm *__tp) _GL_ARG_NONNULL ((1, 3, 4))); # endif _GL_CXXALIAS_SYS (wcsftime, size_t, (wchar_t *__buf, size_t __bufsize, const wchar_t *__fmt, const struct tm *__tp)); # endif _GL_CXXALIASWARN (wcsftime); #elif defined GNULIB_POSIXCHECK # undef wcsftime # if HAVE_RAW_DECL_WCSFTIME _GL_WARN_ON_USE (wcsftime, "wcsftime is unportable - " "use gnulib module wcsftime for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_WCHAR_H */ #endif /* _@GUARD_PREFIX@_WCHAR_H */ #endif gnuastro-0.5/bootstrapped/lib/verify.h0000644000175000017500000002561113217200021015063 00000000000000/* Compile-time assert-like macros. Copyright (C) 2005-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert, Bruno Haible, and Jim Meyering. */ #ifndef _GL_VERIFY_H #define _GL_VERIFY_H /* Define _GL_HAVE__STATIC_ASSERT to 1 if _Static_assert works as per C11. This is supported by GCC 4.6.0 and later, in C mode, and its use here generates easier-to-read diagnostics when verify (R) fails. Define _GL_HAVE_STATIC_ASSERT to 1 if static_assert works as per C++11. This will likely be supported by future GCC versions, in C++ mode. Use this only with GCC. If we were willing to slow 'configure' down we could also use it with other compilers, but since this affects only the quality of diagnostics, why bother? */ #if (4 < __GNUC__ + (6 <= __GNUC_MINOR__) \ && (201112L <= __STDC_VERSION__ || !defined __STRICT_ANSI__) \ && !defined __cplusplus) # define _GL_HAVE__STATIC_ASSERT 1 #endif /* The condition (99 < __GNUC__) is temporary, until we know about the first G++ release that supports static_assert. */ #if (99 < __GNUC__) && defined __cplusplus # define _GL_HAVE_STATIC_ASSERT 1 #endif /* FreeBSD 9.1 , included by and lots of other system headers, defines a conflicting _Static_assert that is no better than ours; override it. */ #ifndef _GL_HAVE_STATIC_ASSERT # include # undef _Static_assert #endif /* Each of these macros verifies that its argument R is nonzero. To be portable, R should be an integer constant expression. Unlike assert (R), there is no run-time overhead. If _Static_assert works, verify (R) uses it directly. Similarly, _GL_VERIFY_TRUE works by packaging a _Static_assert inside a struct that is an operand of sizeof. The code below uses several ideas for C++ compilers, and for C compilers that do not support _Static_assert: * The first step is ((R) ? 1 : -1). Given an expression R, of integral or boolean or floating-point type, this yields an expression of integral type, whose value is later verified to be constant and nonnegative. * Next this expression W is wrapped in a type struct _gl_verify_type { unsigned int _gl_verify_error_if_negative: W; }. If W is negative, this yields a compile-time error. No compiler can deal with a bit-field of negative size. One might think that an array size check would have the same effect, that is, that the type struct { unsigned int dummy[W]; } would work as well. However, inside a function, some compilers (such as C++ compilers and GNU C) allow local parameters and variables inside array size expressions. With these compilers, an array size check would not properly diagnose this misuse of the verify macro: void function (int n) { verify (n < 0); } * For the verify macro, the struct _gl_verify_type will need to somehow be embedded into a declaration. To be portable, this declaration must declare an object, a constant, a function, or a typedef name. If the declared entity uses the type directly, such as in struct dummy {...}; typedef struct {...} dummy; extern struct {...} *dummy; extern void dummy (struct {...} *); extern struct {...} *dummy (void); two uses of the verify macro would yield colliding declarations if the entity names are not disambiguated. A workaround is to attach the current line number to the entity name: #define _GL_CONCAT0(x, y) x##y #define _GL_CONCAT(x, y) _GL_CONCAT0 (x, y) extern struct {...} * _GL_CONCAT (dummy, __LINE__); But this has the problem that two invocations of verify from within the same macro would collide, since the __LINE__ value would be the same for both invocations. (The GCC __COUNTER__ macro solves this problem, but is not portable.) A solution is to use the sizeof operator. It yields a number, getting rid of the identity of the type. Declarations like extern int dummy [sizeof (struct {...})]; extern void dummy (int [sizeof (struct {...})]); extern int (*dummy (void)) [sizeof (struct {...})]; can be repeated. * Should the implementation use a named struct or an unnamed struct? Which of the following alternatives can be used? extern int dummy [sizeof (struct {...})]; extern int dummy [sizeof (struct _gl_verify_type {...})]; extern void dummy (int [sizeof (struct {...})]); extern void dummy (int [sizeof (struct _gl_verify_type {...})]); extern int (*dummy (void)) [sizeof (struct {...})]; extern int (*dummy (void)) [sizeof (struct _gl_verify_type {...})]; In the second and sixth case, the struct type is exported to the outer scope; two such declarations therefore collide. GCC warns about the first, third, and fourth cases. So the only remaining possibility is the fifth case: extern int (*dummy (void)) [sizeof (struct {...})]; * GCC warns about duplicate declarations of the dummy function if -Wredundant-decls is used. GCC 4.3 and later have a builtin __COUNTER__ macro that can let us generate unique identifiers for each dummy function, to suppress this warning. * This implementation exploits the fact that older versions of GCC, which do not support _Static_assert, also do not warn about the last declaration mentioned above. * GCC warns if -Wnested-externs is enabled and verify() is used within a function body; but inside a function, you can always arrange to use verify_expr() instead. * In C++, any struct definition inside sizeof is invalid. Use a template type to work around the problem. */ /* Concatenate two preprocessor tokens. */ #define _GL_CONCAT(x, y) _GL_CONCAT0 (x, y) #define _GL_CONCAT0(x, y) x##y /* _GL_COUNTER is an integer, preferably one that changes each time we use it. Use __COUNTER__ if it works, falling back on __LINE__ otherwise. __LINE__ isn't perfect, but it's better than a constant. */ #if defined __COUNTER__ && __COUNTER__ != __COUNTER__ # define _GL_COUNTER __COUNTER__ #else # define _GL_COUNTER __LINE__ #endif /* Generate a symbol with the given prefix, making it unique if possible. */ #define _GL_GENSYM(prefix) _GL_CONCAT (prefix, _GL_COUNTER) /* Verify requirement R at compile-time, as an integer constant expression that returns 1. If R is false, fail at compile-time, preferably with a diagnostic that includes the string-literal DIAGNOSTIC. */ #define _GL_VERIFY_TRUE(R, DIAGNOSTIC) \ (!!sizeof (_GL_VERIFY_TYPE (R, DIAGNOSTIC))) #ifdef __cplusplus # if !GNULIB_defined_struct__gl_verify_type template struct _gl_verify_type { unsigned int _gl_verify_error_if_negative: w; }; # define GNULIB_defined_struct__gl_verify_type 1 # endif # define _GL_VERIFY_TYPE(R, DIAGNOSTIC) \ _gl_verify_type<(R) ? 1 : -1> #elif defined _GL_HAVE__STATIC_ASSERT # define _GL_VERIFY_TYPE(R, DIAGNOSTIC) \ struct { \ _Static_assert (R, DIAGNOSTIC); \ int _gl_dummy; \ } #else # define _GL_VERIFY_TYPE(R, DIAGNOSTIC) \ struct { unsigned int _gl_verify_error_if_negative: (R) ? 1 : -1; } #endif /* Verify requirement R at compile-time, as a declaration without a trailing ';'. If R is false, fail at compile-time, preferably with a diagnostic that includes the string-literal DIAGNOSTIC. Unfortunately, unlike C11, this implementation must appear as an ordinary declaration, and cannot appear inside struct { ... }. */ #ifdef _GL_HAVE__STATIC_ASSERT # define _GL_VERIFY _Static_assert #else # define _GL_VERIFY(R, DIAGNOSTIC) \ extern int (*_GL_GENSYM (_gl_verify_function) (void)) \ [_GL_VERIFY_TRUE (R, DIAGNOSTIC)] #endif /* _GL_STATIC_ASSERT_H is defined if this code is copied into assert.h. */ #ifdef _GL_STATIC_ASSERT_H # if !defined _GL_HAVE__STATIC_ASSERT && !defined _Static_assert # define _Static_assert(R, DIAGNOSTIC) _GL_VERIFY (R, DIAGNOSTIC) # endif # if !defined _GL_HAVE_STATIC_ASSERT && !defined static_assert # define static_assert _Static_assert /* C11 requires this #define. */ # endif #endif /* @assert.h omit start@ */ /* Each of these macros verifies that its argument R is nonzero. To be portable, R should be an integer constant expression. Unlike assert (R), there is no run-time overhead. There are two macros, since no single macro can be used in all contexts in C. verify_true (R) is for scalar contexts, including integer constant expression contexts. verify (R) is for declaration contexts, e.g., the top level. */ /* Verify requirement R at compile-time, as an integer constant expression. Return 1. This is equivalent to verify_expr (R, 1). verify_true is obsolescent; please use verify_expr instead. */ #define verify_true(R) _GL_VERIFY_TRUE (R, "verify_true (" #R ")") /* Verify requirement R at compile-time. Return the value of the expression E. */ #define verify_expr(R, E) \ (_GL_VERIFY_TRUE (R, "verify_expr (" #R ", " #E ")") ? (E) : (E)) /* Verify requirement R at compile-time, as a declaration without a trailing ';'. */ #ifdef __GNUC__ # define verify(R) _GL_VERIFY (R, "verify (" #R ")") #else /* PGI barfs if R is long. Play it safe. */ # define verify(R) _GL_VERIFY (R, "verify (...)") #endif #ifndef __has_builtin # define __has_builtin(x) 0 #endif /* Assume that R always holds. This lets the compiler optimize accordingly. R should not have side-effects; it may or may not be evaluated. Behavior is undefined if R is false. */ #if (__has_builtin (__builtin_unreachable) \ || 4 < __GNUC__ + (5 <= __GNUC_MINOR__)) # define assume(R) ((R) ? (void) 0 : __builtin_unreachable ()) #elif 1200 <= _MSC_VER # define assume(R) __assume (R) #elif ((defined GCC_LINT || defined lint) \ && (__has_builtin (__builtin_trap) \ || 3 < __GNUC__ + (3 < __GNUC_MINOR__ + (4 <= __GNUC_PATCHLEVEL__)))) /* Doing it this way helps various packages when configured with --enable-gcc-warnings, which compiles with -Dlint. It's nicer when 'assume' silences warnings even with older GCCs. */ # define assume(R) ((R) ? (void) 0 : __builtin_trap ()) #else # define assume(R) ((void) (0 && (R))) #endif /* @assert.h omit end@ */ #endif gnuastro-0.5/bootstrapped/lib/vasnprintf.h0000644000175000017500000000560113217200021015746 00000000000000/* vsprintf with automatic memory allocation. Copyright (C) 2002-2004, 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _VASNPRINTF_H #define _VASNPRINTF_H /* Get va_list. */ #include /* Get size_t. */ #include /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif #ifdef __cplusplus extern "C" { #endif /* Write formatted output to a string dynamically allocated with malloc(). You can pass a preallocated buffer for the result in RESULTBUF and its size in *LENGTHP; otherwise you pass RESULTBUF = NULL. If successful, return the address of the string (this may be = RESULTBUF if no dynamic memory allocation was necessary) and set *LENGTHP to the number of resulting bytes, excluding the trailing NUL. Upon error, set errno and return NULL. When dynamic memory allocation occurs, the preallocated buffer is left alone (with possibly modified contents). This makes it possible to use a statically allocated or stack-allocated buffer, like this: char buf[100]; size_t len = sizeof (buf); char *output = vasnprintf (buf, &len, format, args); if (output == NULL) ... error handling ...; else { ... use the output string ...; if (output != buf) free (output); } */ #if REPLACE_VASNPRINTF # define asnprintf rpl_asnprintf # define vasnprintf rpl_vasnprintf #endif extern char * asnprintf (char *resultbuf, size_t *lengthp, const char *format, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 3, 4)); extern char * vasnprintf (char *resultbuf, size_t *lengthp, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT ((__printf__, 3, 0)); #ifdef __cplusplus } #endif #endif /* _VASNPRINTF_H */ gnuastro-0.5/bootstrapped/lib/printf-parse.h0000644000175000017500000001216413217200021016170 00000000000000/* Parse printf format string. Copyright (C) 1999, 2002-2003, 2005, 2007, 2010-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _PRINTF_PARSE_H #define _PRINTF_PARSE_H /* This file can be parametrized with the following macros: ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. STATIC Set to 'static' to declare the function static. */ #if HAVE_FEATURES_H # include /* for __GLIBC__, __UCLIBC__ */ #endif #include "printf-args.h" /* Flags */ #define FLAG_GROUP 1 /* ' flag */ #define FLAG_LEFT 2 /* - flag */ #define FLAG_SHOWSIGN 4 /* + flag */ #define FLAG_SPACE 8 /* space flag */ #define FLAG_ALT 16 /* # flag */ #define FLAG_ZERO 32 #if __GLIBC__ >= 2 && !defined __UCLIBC__ # define FLAG_LOCALIZED 64 /* I flag, uses localized digits */ #endif /* arg_index value indicating that no argument is consumed. */ #define ARG_NONE (~(size_t)0) /* xxx_directive: A parsed directive. xxx_directives: A parsed format string. */ /* Number of directly allocated directives (no malloc() needed). */ #define N_DIRECT_ALLOC_DIRECTIVES 7 /* A parsed directive. */ typedef struct { const char* dir_start; const char* dir_end; int flags; const char* width_start; const char* width_end; size_t width_arg_index; const char* precision_start; const char* precision_end; size_t precision_arg_index; char conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } char_directive; /* A parsed format string. */ typedef struct { size_t count; char_directive *dir; size_t max_width_length; size_t max_precision_length; char_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } char_directives; #if ENABLE_UNISTDIO /* A parsed directive. */ typedef struct { const uint8_t* dir_start; const uint8_t* dir_end; int flags; const uint8_t* width_start; const uint8_t* width_end; size_t width_arg_index; const uint8_t* precision_start; const uint8_t* precision_end; size_t precision_arg_index; uint8_t conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } u8_directive; /* A parsed format string. */ typedef struct { size_t count; u8_directive *dir; size_t max_width_length; size_t max_precision_length; u8_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } u8_directives; /* A parsed directive. */ typedef struct { const uint16_t* dir_start; const uint16_t* dir_end; int flags; const uint16_t* width_start; const uint16_t* width_end; size_t width_arg_index; const uint16_t* precision_start; const uint16_t* precision_end; size_t precision_arg_index; uint16_t conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } u16_directive; /* A parsed format string. */ typedef struct { size_t count; u16_directive *dir; size_t max_width_length; size_t max_precision_length; u16_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } u16_directives; /* A parsed directive. */ typedef struct { const uint32_t* dir_start; const uint32_t* dir_end; int flags; const uint32_t* width_start; const uint32_t* width_end; size_t width_arg_index; const uint32_t* precision_start; const uint32_t* precision_end; size_t precision_arg_index; uint32_t conversion; /* d i o u x X f F e E g G a A c s p n U % but not C S */ size_t arg_index; } u32_directive; /* A parsed format string. */ typedef struct { size_t count; u32_directive *dir; size_t max_width_length; size_t max_precision_length; u32_directive direct_alloc_dir[N_DIRECT_ALLOC_DIRECTIVES]; } u32_directives; #endif /* Parses the format string. Fills in the number N of directives, and fills in directives[0], ..., directives[N-1], and sets directives[N].dir_start to the end of the format string. Also fills in the arg_type fields of the arguments and the needed count of arguments. */ #if ENABLE_UNISTDIO extern int ulc_printf_parse (const char *format, char_directives *d, arguments *a); extern int u8_printf_parse (const uint8_t *format, u8_directives *d, arguments *a); extern int u16_printf_parse (const uint16_t *format, u16_directives *d, arguments *a); extern int u32_printf_parse (const uint32_t *format, u32_directives *d, arguments *a); #else # ifdef STATIC STATIC # else extern # endif int printf_parse (const char *format, char_directives *d, arguments *a); #endif #endif /* _PRINTF_PARSE_H */ gnuastro-0.5/bootstrapped/lib/printf-args.h0000644000175000017500000000753413217200021016017 00000000000000/* Decomposed printf argument list. Copyright (C) 1999, 2002-2003, 2006-2007, 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _PRINTF_ARGS_H #define _PRINTF_ARGS_H /* This file can be parametrized with the following macros: ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. PRINTF_FETCHARGS Name of the function to be declared. STATIC Set to 'static' to declare the function static. */ /* Default parameters. */ #ifndef PRINTF_FETCHARGS # define PRINTF_FETCHARGS printf_fetchargs #endif /* Get size_t. */ #include /* Get wchar_t. */ #if HAVE_WCHAR_T # include #endif /* Get wint_t. */ #if HAVE_WINT_T # include #endif /* Get va_list. */ #include /* Argument types */ typedef enum { TYPE_NONE, TYPE_SCHAR, TYPE_UCHAR, TYPE_SHORT, TYPE_USHORT, TYPE_INT, TYPE_UINT, TYPE_LONGINT, TYPE_ULONGINT, #if HAVE_LONG_LONG_INT TYPE_LONGLONGINT, TYPE_ULONGLONGINT, #endif TYPE_DOUBLE, TYPE_LONGDOUBLE, TYPE_CHAR, #if HAVE_WINT_T TYPE_WIDE_CHAR, #endif TYPE_STRING, #if HAVE_WCHAR_T TYPE_WIDE_STRING, #endif TYPE_POINTER, TYPE_COUNT_SCHAR_POINTER, TYPE_COUNT_SHORT_POINTER, TYPE_COUNT_INT_POINTER, TYPE_COUNT_LONGINT_POINTER #if HAVE_LONG_LONG_INT , TYPE_COUNT_LONGLONGINT_POINTER #endif #if ENABLE_UNISTDIO /* The unistdio extensions. */ , TYPE_U8_STRING , TYPE_U16_STRING , TYPE_U32_STRING #endif } arg_type; /* Polymorphic argument */ typedef struct { arg_type type; union { signed char a_schar; unsigned char a_uchar; short a_short; unsigned short a_ushort; int a_int; unsigned int a_uint; long int a_longint; unsigned long int a_ulongint; #if HAVE_LONG_LONG_INT long long int a_longlongint; unsigned long long int a_ulonglongint; #endif float a_float; double a_double; long double a_longdouble; int a_char; #if HAVE_WINT_T wint_t a_wide_char; #endif const char* a_string; #if HAVE_WCHAR_T const wchar_t* a_wide_string; #endif void* a_pointer; signed char * a_count_schar_pointer; short * a_count_short_pointer; int * a_count_int_pointer; long int * a_count_longint_pointer; #if HAVE_LONG_LONG_INT long long int * a_count_longlongint_pointer; #endif #if ENABLE_UNISTDIO /* The unistdio extensions. */ const uint8_t * a_u8_string; const uint16_t * a_u16_string; const uint32_t * a_u32_string; #endif } a; } argument; /* Number of directly allocated arguments (no malloc() needed). */ #define N_DIRECT_ALLOC_ARGUMENTS 7 typedef struct { size_t count; argument *arg; argument direct_alloc_arg[N_DIRECT_ALLOC_ARGUMENTS]; } arguments; /* Fetch the arguments, putting them into a. */ #ifdef STATIC STATIC #else extern #endif int PRINTF_FETCHARGS (va_list args, arguments *a); #endif /* _PRINTF_ARGS_H */ gnuastro-0.5/bootstrapped/lib/float+.h0000644000175000017500000001274613217200021014744 00000000000000/* Supplemental information about the floating-point formats. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _FLOATPLUS_H #define _FLOATPLUS_H #include #include /* Number of bits in the mantissa of a floating-point number, including the "hidden bit". */ #if FLT_RADIX == 2 # define FLT_MANT_BIT FLT_MANT_DIG # define DBL_MANT_BIT DBL_MANT_DIG # define LDBL_MANT_BIT LDBL_MANT_DIG #elif FLT_RADIX == 4 # define FLT_MANT_BIT (FLT_MANT_DIG * 2) # define DBL_MANT_BIT (DBL_MANT_DIG * 2) # define LDBL_MANT_BIT (LDBL_MANT_DIG * 2) #elif FLT_RADIX == 16 # define FLT_MANT_BIT (FLT_MANT_DIG * 4) # define DBL_MANT_BIT (DBL_MANT_DIG * 4) # define LDBL_MANT_BIT (LDBL_MANT_DIG * 4) #endif /* Bit mask that can be used to mask the exponent, as an unsigned number. */ #define FLT_EXP_MASK ((FLT_MAX_EXP - FLT_MIN_EXP) | 7) #define DBL_EXP_MASK ((DBL_MAX_EXP - DBL_MIN_EXP) | 7) #define LDBL_EXP_MASK ((LDBL_MAX_EXP - LDBL_MIN_EXP) | 7) /* Number of bits used for the exponent of a floating-point number, including the exponent's sign. */ #define FLT_EXP_BIT \ (FLT_EXP_MASK < 0x100 ? 8 : \ FLT_EXP_MASK < 0x200 ? 9 : \ FLT_EXP_MASK < 0x400 ? 10 : \ FLT_EXP_MASK < 0x800 ? 11 : \ FLT_EXP_MASK < 0x1000 ? 12 : \ FLT_EXP_MASK < 0x2000 ? 13 : \ FLT_EXP_MASK < 0x4000 ? 14 : \ FLT_EXP_MASK < 0x8000 ? 15 : \ FLT_EXP_MASK < 0x10000 ? 16 : \ FLT_EXP_MASK < 0x20000 ? 17 : \ FLT_EXP_MASK < 0x40000 ? 18 : \ FLT_EXP_MASK < 0x80000 ? 19 : \ FLT_EXP_MASK < 0x100000 ? 20 : \ FLT_EXP_MASK < 0x200000 ? 21 : \ FLT_EXP_MASK < 0x400000 ? 22 : \ FLT_EXP_MASK < 0x800000 ? 23 : \ FLT_EXP_MASK < 0x1000000 ? 24 : \ FLT_EXP_MASK < 0x2000000 ? 25 : \ FLT_EXP_MASK < 0x4000000 ? 26 : \ FLT_EXP_MASK < 0x8000000 ? 27 : \ FLT_EXP_MASK < 0x10000000 ? 28 : \ FLT_EXP_MASK < 0x20000000 ? 29 : \ FLT_EXP_MASK < 0x40000000 ? 30 : \ FLT_EXP_MASK <= 0x7fffffff ? 31 : \ 32) #define DBL_EXP_BIT \ (DBL_EXP_MASK < 0x100 ? 8 : \ DBL_EXP_MASK < 0x200 ? 9 : \ DBL_EXP_MASK < 0x400 ? 10 : \ DBL_EXP_MASK < 0x800 ? 11 : \ DBL_EXP_MASK < 0x1000 ? 12 : \ DBL_EXP_MASK < 0x2000 ? 13 : \ DBL_EXP_MASK < 0x4000 ? 14 : \ DBL_EXP_MASK < 0x8000 ? 15 : \ DBL_EXP_MASK < 0x10000 ? 16 : \ DBL_EXP_MASK < 0x20000 ? 17 : \ DBL_EXP_MASK < 0x40000 ? 18 : \ DBL_EXP_MASK < 0x80000 ? 19 : \ DBL_EXP_MASK < 0x100000 ? 20 : \ DBL_EXP_MASK < 0x200000 ? 21 : \ DBL_EXP_MASK < 0x400000 ? 22 : \ DBL_EXP_MASK < 0x800000 ? 23 : \ DBL_EXP_MASK < 0x1000000 ? 24 : \ DBL_EXP_MASK < 0x2000000 ? 25 : \ DBL_EXP_MASK < 0x4000000 ? 26 : \ DBL_EXP_MASK < 0x8000000 ? 27 : \ DBL_EXP_MASK < 0x10000000 ? 28 : \ DBL_EXP_MASK < 0x20000000 ? 29 : \ DBL_EXP_MASK < 0x40000000 ? 30 : \ DBL_EXP_MASK <= 0x7fffffff ? 31 : \ 32) #define LDBL_EXP_BIT \ (LDBL_EXP_MASK < 0x100 ? 8 : \ LDBL_EXP_MASK < 0x200 ? 9 : \ LDBL_EXP_MASK < 0x400 ? 10 : \ LDBL_EXP_MASK < 0x800 ? 11 : \ LDBL_EXP_MASK < 0x1000 ? 12 : \ LDBL_EXP_MASK < 0x2000 ? 13 : \ LDBL_EXP_MASK < 0x4000 ? 14 : \ LDBL_EXP_MASK < 0x8000 ? 15 : \ LDBL_EXP_MASK < 0x10000 ? 16 : \ LDBL_EXP_MASK < 0x20000 ? 17 : \ LDBL_EXP_MASK < 0x40000 ? 18 : \ LDBL_EXP_MASK < 0x80000 ? 19 : \ LDBL_EXP_MASK < 0x100000 ? 20 : \ LDBL_EXP_MASK < 0x200000 ? 21 : \ LDBL_EXP_MASK < 0x400000 ? 22 : \ LDBL_EXP_MASK < 0x800000 ? 23 : \ LDBL_EXP_MASK < 0x1000000 ? 24 : \ LDBL_EXP_MASK < 0x2000000 ? 25 : \ LDBL_EXP_MASK < 0x4000000 ? 26 : \ LDBL_EXP_MASK < 0x8000000 ? 27 : \ LDBL_EXP_MASK < 0x10000000 ? 28 : \ LDBL_EXP_MASK < 0x20000000 ? 29 : \ LDBL_EXP_MASK < 0x40000000 ? 30 : \ LDBL_EXP_MASK <= 0x7fffffff ? 31 : \ 32) /* Number of bits used for a floating-point number: the mantissa (not counting the "hidden bit", since it may or may not be explicit), the exponent, and the sign. */ #define FLT_TOTAL_BIT ((FLT_MANT_BIT - 1) + FLT_EXP_BIT + 1) #define DBL_TOTAL_BIT ((DBL_MANT_BIT - 1) + DBL_EXP_BIT + 1) #define LDBL_TOTAL_BIT ((LDBL_MANT_BIT - 1) + LDBL_EXP_BIT + 1) /* Number of bytes used for a floating-point number. This can be smaller than the 'sizeof'. For example, on i386 systems, 'long double' most often have LDBL_MANT_BIT = 64, LDBL_EXP_BIT = 16, hence LDBL_TOTAL_BIT = 80 bits, i.e. 10 bytes of consecutive memory, but sizeof (long double) = 12 or = 16. */ #define SIZEOF_FLT ((FLT_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) #define SIZEOF_DBL ((DBL_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) #define SIZEOF_LDBL ((LDBL_TOTAL_BIT + CHAR_BIT - 1) / CHAR_BIT) /* Verify that SIZEOF_FLT <= sizeof (float) etc. */ typedef int verify_sizeof_flt[SIZEOF_FLT <= sizeof (float) ? 1 : -1]; typedef int verify_sizeof_dbl[SIZEOF_DBL <= sizeof (double) ? 1 : - 1]; typedef int verify_sizeof_ldbl[SIZEOF_LDBL <= sizeof (long double) ? 1 : - 1]; #endif /* _FLOATPLUS_H */ gnuastro-0.5/bootstrapped/lib/uniwidth.in.h0000644000175000017500000000411213217200021016010 00000000000000/* Display width functions. Copyright (C) 2001-2002, 2005, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _UNIWIDTH_H #define _UNIWIDTH_H #include "unitypes.h" /* Get size_t. */ #include /* Get locale_charset() declaration. */ #include "localcharset.h" #ifdef __cplusplus extern "C" { #endif /* Display width. */ /* These functions are locale dependent. The encoding argument identifies the encoding (e.g. "ISO-8859-2" for Polish). */ /* Determine number of column positions required for UC. */ extern int uc_width (ucs4_t uc, const char *encoding) _UC_ATTRIBUTE_PURE; /* Determine number of column positions required for first N units (or fewer if S ends before this) in S. */ extern int u8_width (const uint8_t *s, size_t n, const char *encoding) _UC_ATTRIBUTE_PURE; extern int u16_width (const uint16_t *s, size_t n, const char *encoding) _UC_ATTRIBUTE_PURE; extern int u32_width (const uint32_t *s, size_t n, const char *encoding) _UC_ATTRIBUTE_PURE; /* Determine number of column positions required for S. */ extern int u8_strwidth (const uint8_t *s, const char *encoding) _UC_ATTRIBUTE_PURE; extern int u16_strwidth (const uint16_t *s, const char *encoding) _UC_ATTRIBUTE_PURE; extern int u32_strwidth (const uint32_t *s, const char *encoding) _UC_ATTRIBUTE_PURE; #ifdef __cplusplus } #endif #endif /* _UNIWIDTH_H */ gnuastro-0.5/bootstrapped/lib/unitypes.in.h0000644000175000017500000000316413217200021016043 00000000000000/* Elementary types and macros for the GNU UniString library. Copyright (C) 2002, 2005-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _UNITYPES_H #define _UNITYPES_H /* Get uint8_t, uint16_t, uint32_t. */ #include /* Type representing a Unicode character. */ typedef uint32_t ucs4_t; /* Attribute of a function whose result depends only on the arguments (not pointers!) and which has no side effects. */ #ifndef _UC_ATTRIBUTE_CONST # if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 95) # define _UC_ATTRIBUTE_CONST __attribute__ ((__const__)) # else # define _UC_ATTRIBUTE_CONST # endif #endif /* Attribute of a function whose result depends only on the arguments (possibly pointers) and global memory, and which has no side effects. */ #ifndef _UC_ATTRIBUTE_PURE # if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _UC_ATTRIBUTE_PURE __attribute__ ((__pure__)) # else # define _UC_ATTRIBUTE_PURE # endif #endif #endif /* _UNITYPES_H */ gnuastro-0.5/bootstrapped/lib/unistd.in.h0000644000175000017500000015426713217200021015504 00000000000000/* Substitute for and wrapper around . Copyright (C) 2003-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_UNISTD_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #ifdef _GL_INCLUDING_UNISTD_H /* Special invocation convention: - On Mac OS X 10.3.9 we have a sequence of nested includes -> -> -> In this situation, the functions are not yet declared, therefore we cannot provide the C++ aliases. */ #@INCLUDE_NEXT@ @NEXT_UNISTD_H@ #else /* Normal invocation convention. */ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_UNISTD_H@ # define _GL_INCLUDING_UNISTD_H # @INCLUDE_NEXT@ @NEXT_UNISTD_H@ # undef _GL_INCLUDING_UNISTD_H #endif /* Get all possible declarations of gethostname(). */ #if @GNULIB_GETHOSTNAME@ && @UNISTD_H_HAVE_WINSOCK2_H@ \ && !defined _GL_INCLUDING_WINSOCK2_H # define _GL_INCLUDING_WINSOCK2_H # include # undef _GL_INCLUDING_WINSOCK2_H #endif #if !defined _@GUARD_PREFIX@_UNISTD_H && !defined _GL_INCLUDING_WINSOCK2_H #define _@GUARD_PREFIX@_UNISTD_H /* NetBSD 5.0 mis-defines NULL. Also get size_t. */ #include /* mingw doesn't define the SEEK_* or *_FILENO macros in . */ /* MSVC declares 'unlink' in , not in . We must include it before we #define unlink rpl_unlink. */ /* Cygwin 1.7.1 declares symlinkat in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if (!(defined SEEK_CUR && defined SEEK_END && defined SEEK_SET) \ || ((@GNULIB_UNLINK@ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__)) \ || ((@GNULIB_SYMLINKAT@ || defined GNULIB_POSIXCHECK) \ && defined __CYGWIN__)) \ && ! defined __GLIBC__ # include #endif /* Cygwin 1.7.1 declares unlinkat in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if (@GNULIB_UNLINKAT@ || defined GNULIB_POSIXCHECK) && defined __CYGWIN__ \ && ! defined __GLIBC__ # include #endif /* mingw fails to declare _exit in . */ /* mingw, MSVC, BeOS, Haiku declare environ in , not in . */ /* Solaris declares getcwd not only in but also in . */ /* OSF Tru64 Unix cannot see gnulib rpl_strtod when system is included here. */ /* But avoid namespace pollution on glibc systems. */ #if !defined __GLIBC__ && !defined __osf__ # define __need_system_stdlib_h # include # undef __need_system_stdlib_h #endif /* Native Windows platforms declare chdir, getcwd, rmdir in and/or , not in . They also declare access(), chmod(), close(), dup(), dup2(), isatty(), lseek(), read(), unlink(), write() in . */ #if ((@GNULIB_CHDIR@ || @GNULIB_GETCWD@ || @GNULIB_RMDIR@ \ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__)) # include /* mingw32, mingw64 */ # include /* mingw64, MSVC 9 */ #elif (@GNULIB_CLOSE@ || @GNULIB_DUP@ || @GNULIB_DUP2@ || @GNULIB_ISATTY@ \ || @GNULIB_LSEEK@ || @GNULIB_READ@ || @GNULIB_UNLINK@ || @GNULIB_WRITE@ \ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif /* AIX and OSF/1 5.1 declare getdomainname in , not in . NonStop Kernel declares gethostname in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if ((@GNULIB_GETDOMAINNAME@ && (defined _AIX || defined __osf__)) \ || (@GNULIB_GETHOSTNAME@ && defined __TANDEM)) \ && !defined __GLIBC__ # include #endif /* MSVC defines off_t in . May also define off_t to a 64-bit type on native Windows. */ #if !@HAVE_UNISTD_H@ || @WINDOWS_64_BIT_OFF_T@ /* Get off_t. */ # include #endif #if (@GNULIB_READ@ || @GNULIB_WRITE@ \ || @GNULIB_READLINK@ || @GNULIB_READLINKAT@ \ || @GNULIB_PREAD@ || @GNULIB_PWRITE@ || defined GNULIB_POSIXCHECK) /* Get ssize_t. */ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Get getopt(), optarg, optind, opterr, optopt. */ #if @GNULIB_UNISTD_H_GETOPT@ && !defined _GL_SYSTEM_GETOPT # include # include #endif #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_UNISTD_INLINE # define _GL_UNISTD_INLINE _GL_INLINE #endif /* Hide some function declarations from . */ #if @GNULIB_GETHOSTNAME@ && @UNISTD_H_HAVE_WINSOCK2_H@ # if !defined _@GUARD_PREFIX@_SYS_SOCKET_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef socket # define socket socket_used_without_including_sys_socket_h # undef connect # define connect connect_used_without_including_sys_socket_h # undef accept # define accept accept_used_without_including_sys_socket_h # undef bind # define bind bind_used_without_including_sys_socket_h # undef getpeername # define getpeername getpeername_used_without_including_sys_socket_h # undef getsockname # define getsockname getsockname_used_without_including_sys_socket_h # undef getsockopt # define getsockopt getsockopt_used_without_including_sys_socket_h # undef listen # define listen listen_used_without_including_sys_socket_h # undef recv # define recv recv_used_without_including_sys_socket_h # undef send # define send send_used_without_including_sys_socket_h # undef recvfrom # define recvfrom recvfrom_used_without_including_sys_socket_h # undef sendto # define sendto sendto_used_without_including_sys_socket_h # undef setsockopt # define setsockopt setsockopt_used_without_including_sys_socket_h # undef shutdown # define shutdown shutdown_used_without_including_sys_socket_h # else _GL_WARN_ON_USE (socket, "socket() used without including "); _GL_WARN_ON_USE (connect, "connect() used without including "); _GL_WARN_ON_USE (accept, "accept() used without including "); _GL_WARN_ON_USE (bind, "bind() used without including "); _GL_WARN_ON_USE (getpeername, "getpeername() used without including "); _GL_WARN_ON_USE (getsockname, "getsockname() used without including "); _GL_WARN_ON_USE (getsockopt, "getsockopt() used without including "); _GL_WARN_ON_USE (listen, "listen() used without including "); _GL_WARN_ON_USE (recv, "recv() used without including "); _GL_WARN_ON_USE (send, "send() used without including "); _GL_WARN_ON_USE (recvfrom, "recvfrom() used without including "); _GL_WARN_ON_USE (sendto, "sendto() used without including "); _GL_WARN_ON_USE (setsockopt, "setsockopt() used without including "); _GL_WARN_ON_USE (shutdown, "shutdown() used without including "); # endif # endif # if !defined _@GUARD_PREFIX@_SYS_SELECT_H # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef select # define select select_used_without_including_sys_select_h # else _GL_WARN_ON_USE (select, "select() used without including "); # endif # endif #endif /* OS/2 EMX lacks these macros. */ #ifndef STDIN_FILENO # define STDIN_FILENO 0 #endif #ifndef STDOUT_FILENO # define STDOUT_FILENO 1 #endif #ifndef STDERR_FILENO # define STDERR_FILENO 2 #endif /* Ensure *_OK macros exist. */ #ifndef F_OK # define F_OK 0 # define X_OK 1 # define W_OK 2 # define R_OK 4 #endif /* Declare overridden functions. */ #if defined GNULIB_POSIXCHECK /* The access() function is a security risk. */ _GL_WARN_ON_USE (access, "the access function is a security risk - " "use the gnulib module faccessat instead"); #endif #if @GNULIB_CHDIR@ _GL_CXXALIAS_SYS (chdir, int, (const char *file) _GL_ARG_NONNULL ((1))); _GL_CXXALIASWARN (chdir); #elif defined GNULIB_POSIXCHECK # undef chdir # if HAVE_RAW_DECL_CHDIR _GL_WARN_ON_USE (chown, "chdir is not always in - " "use gnulib module chdir for portability"); # endif #endif #if @GNULIB_CHOWN@ /* Change the owner of FILE to UID (if UID is not -1) and the group of FILE to GID (if GID is not -1). Follow symbolic links. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_DUP2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define dup2 rpl_dup2 # endif _GL_FUNCDECL_RPL (dup2, int, (int oldfd, int newfd)); _GL_CXXALIAS_RPL (dup2, int, (int oldfd, int newfd)); # else # if !@HAVE_DUP2@ _GL_FUNCDECL_SYS (dup2, int, (int oldfd, int newfd)); # endif _GL_CXXALIAS_SYS (dup2, int, (int oldfd, int newfd)); # endif _GL_CXXALIASWARN (dup2); #elif defined GNULIB_POSIXCHECK # undef dup2 # if HAVE_RAW_DECL_DUP2 _GL_WARN_ON_USE (dup2, "dup2 is unportable - " "use gnulib module dup2 for portability"); # endif #endif #if @GNULIB_DUP3@ /* Copy the file descriptor OLDFD into file descriptor NEWFD, with the specified flags. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). Close NEWFD first if it is open. Return newfd if successful, otherwise -1 and errno set. See the Linux man page at . */ # if @HAVE_DUP3@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define dup3 rpl_dup3 # endif _GL_FUNCDECL_RPL (dup3, int, (int oldfd, int newfd, int flags)); _GL_CXXALIAS_RPL (dup3, int, (int oldfd, int newfd, int flags)); # else _GL_FUNCDECL_SYS (dup3, int, (int oldfd, int newfd, int flags)); _GL_CXXALIAS_SYS (dup3, int, (int oldfd, int newfd, int flags)); # endif _GL_CXXALIASWARN (dup3); #elif defined GNULIB_POSIXCHECK # undef dup3 # if HAVE_RAW_DECL_DUP3 _GL_WARN_ON_USE (dup3, "dup3 is unportable - " "use gnulib module dup3 for portability"); # endif #endif #if @GNULIB_ENVIRON@ # if !@HAVE_DECL_ENVIRON@ /* Set of environment variables and values. An array of strings of the form "VARIABLE=VALUE", terminated with a NULL. */ # if defined __APPLE__ && defined __MACH__ # include # if !TARGET_OS_IPHONE && !TARGET_IPHONE_SIMULATOR # define _GL_USE_CRT_EXTERNS # endif # endif # ifdef _GL_USE_CRT_EXTERNS # include # define environ (*_NSGetEnviron ()) # else # ifdef __cplusplus extern "C" { # endif extern char **environ; # ifdef __cplusplus } # endif # endif # endif #elif defined GNULIB_POSIXCHECK # if HAVE_RAW_DECL_ENVIRON _GL_UNISTD_INLINE char *** rpl_environ (void) { return &environ; } _GL_WARN_ON_USE (rpl_environ, "environ is unportable - " "use gnulib module environ for portability"); # undef environ # define environ (*rpl_environ ()) # endif #endif #if @GNULIB_EUIDACCESS@ /* Like access(), except that it uses the effective user id and group id of the current process. */ # if !@HAVE_EUIDACCESS@ _GL_FUNCDECL_SYS (euidaccess, int, (const char *filename, int mode) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (euidaccess, int, (const char *filename, int mode)); _GL_CXXALIASWARN (euidaccess); # if defined GNULIB_POSIXCHECK /* Like access(), this function is a security risk. */ _GL_WARN_ON_USE (euidaccess, "the euidaccess function is a security risk - " "use the gnulib module faccessat instead"); # endif #elif defined GNULIB_POSIXCHECK # undef euidaccess # if HAVE_RAW_DECL_EUIDACCESS _GL_WARN_ON_USE (euidaccess, "euidaccess is unportable - " "use gnulib module euidaccess for portability"); # endif #endif #if @GNULIB_FACCESSAT@ # if @REPLACE_FACCESSAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef faccessat # define faccessat rpl_faccessat # endif _GL_FUNCDECL_RPL (faccessat, int, (int fd, char const *name, int mode, int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (faccessat, int, (int fd, char const *name, int mode, int flag)); # else # if !@HAVE_FACCESSAT@ _GL_FUNCDECL_SYS (faccessat, int, (int fd, char const *file, int mode, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (faccessat, int, (int fd, char const *file, int mode, int flag)); # endif _GL_CXXALIASWARN (faccessat); #elif defined GNULIB_POSIXCHECK # undef faccessat # if HAVE_RAW_DECL_FACCESSAT _GL_WARN_ON_USE (faccessat, "faccessat is not portable - " "use gnulib module faccessat for portability"); # endif #endif #if @GNULIB_FCHDIR@ /* Change the process' current working directory to the directory on which the given file descriptor is open. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if ! @HAVE_FCHDIR@ _GL_FUNCDECL_SYS (fchdir, int, (int /*fd*/)); /* Gnulib internal hooks needed to maintain the fchdir metadata. */ _GL_EXTERN_C int _gl_register_fd (int fd, const char *filename) _GL_ARG_NONNULL ((2)); _GL_EXTERN_C void _gl_unregister_fd (int fd); _GL_EXTERN_C int _gl_register_dup (int oldfd, int newfd); _GL_EXTERN_C const char *_gl_directory_name (int fd); # else # if !@HAVE_DECL_FCHDIR@ _GL_FUNCDECL_SYS (fchdir, int, (int /*fd*/)); # endif # endif _GL_CXXALIAS_SYS (fchdir, int, (int /*fd*/)); _GL_CXXALIASWARN (fchdir); #elif defined GNULIB_POSIXCHECK # undef fchdir # if HAVE_RAW_DECL_FCHDIR _GL_WARN_ON_USE (fchdir, "fchdir is unportable - " "use gnulib module fchdir for portability"); # endif #endif #if @GNULIB_FCHOWNAT@ # if @REPLACE_FCHOWNAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fchownat # define fchownat rpl_fchownat # endif _GL_FUNCDECL_RPL (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag)); # else # if !@HAVE_FCHOWNAT@ _GL_FUNCDECL_SYS (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (fchownat, int, (int fd, char const *file, uid_t owner, gid_t group, int flag)); # endif _GL_CXXALIASWARN (fchownat); #elif defined GNULIB_POSIXCHECK # undef fchownat # if HAVE_RAW_DECL_FCHOWNAT _GL_WARN_ON_USE (fchownat, "fchownat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_FDATASYNC@ /* Synchronize changes to a file. Return 0 if successful, otherwise -1 and errno set. See POSIX:2008 specification . */ # if !@HAVE_FDATASYNC@ || !@HAVE_DECL_FDATASYNC@ _GL_FUNCDECL_SYS (fdatasync, int, (int fd)); # endif _GL_CXXALIAS_SYS (fdatasync, int, (int fd)); _GL_CXXALIASWARN (fdatasync); #elif defined GNULIB_POSIXCHECK # undef fdatasync # if HAVE_RAW_DECL_FDATASYNC _GL_WARN_ON_USE (fdatasync, "fdatasync is unportable - " "use gnulib module fdatasync for portability"); # endif #endif #if @GNULIB_FSYNC@ /* Synchronize changes, including metadata, to a file. Return 0 if successful, otherwise -1 and errno set. See POSIX:2008 specification . */ # if !@HAVE_FSYNC@ _GL_FUNCDECL_SYS (fsync, int, (int fd)); # endif _GL_CXXALIAS_SYS (fsync, int, (int fd)); _GL_CXXALIASWARN (fsync); #elif defined GNULIB_POSIXCHECK # undef fsync # if HAVE_RAW_DECL_FSYNC _GL_WARN_ON_USE (fsync, "fsync is unportable - " "use gnulib module fsync for portability"); # endif #endif #if @GNULIB_FTRUNCATE@ /* Change the size of the file to which FD is opened to become equal to LENGTH. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_FTRUNCATE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ftruncate # define ftruncate rpl_ftruncate # endif _GL_FUNCDECL_RPL (ftruncate, int, (int fd, off_t length)); _GL_CXXALIAS_RPL (ftruncate, int, (int fd, off_t length)); # else # if !@HAVE_FTRUNCATE@ _GL_FUNCDECL_SYS (ftruncate, int, (int fd, off_t length)); # endif _GL_CXXALIAS_SYS (ftruncate, int, (int fd, off_t length)); # endif _GL_CXXALIASWARN (ftruncate); #elif defined GNULIB_POSIXCHECK # undef ftruncate # if HAVE_RAW_DECL_FTRUNCATE _GL_WARN_ON_USE (ftruncate, "ftruncate is unportable - " "use gnulib module ftruncate for portability"); # endif #endif #if @GNULIB_GETCWD@ /* Get the name of the current working directory, and put it in SIZE bytes of BUF. Return BUF if successful, or NULL if the directory couldn't be determined or SIZE was too small. See the POSIX:2008 specification . Additionally, the gnulib module 'getcwd' guarantees the following GNU extension: If BUF is NULL, an array is allocated with 'malloc'; the array is SIZE bytes long, unless SIZE == 0, in which case it is as big as necessary. */ # if @REPLACE_GETCWD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getcwd rpl_getcwd # endif _GL_FUNCDECL_RPL (getcwd, char *, (char *buf, size_t size)); _GL_CXXALIAS_RPL (getcwd, char *, (char *buf, size_t size)); # else /* Need to cast, because on mingw, the second parameter is int size. */ _GL_CXXALIAS_SYS_CAST (getcwd, char *, (char *buf, size_t size)); # endif _GL_CXXALIASWARN (getcwd); #elif defined GNULIB_POSIXCHECK # undef getcwd # if HAVE_RAW_DECL_GETCWD _GL_WARN_ON_USE (getcwd, "getcwd is unportable - " "use gnulib module getcwd for portability"); # endif #endif #if @GNULIB_GETDOMAINNAME@ /* Return the NIS domain name of the machine. WARNING! The NIS domain name is unrelated to the fully qualified host name of the machine. It is also unrelated to email addresses. WARNING! The NIS domain name is usually the empty string or "(none)" when not using NIS. Put up to LEN bytes of the NIS domain name into NAME. Null terminate it if the name is shorter than LEN. If the NIS domain name is longer than LEN, set errno = EINVAL and return -1. Return 0 if successful, otherwise set errno and return -1. */ # if @REPLACE_GETDOMAINNAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getdomainname # define getdomainname rpl_getdomainname # endif _GL_FUNCDECL_RPL (getdomainname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (getdomainname, int, (char *name, size_t len)); # else # if !@HAVE_DECL_GETDOMAINNAME@ _GL_FUNCDECL_SYS (getdomainname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (getdomainname, int, (char *name, size_t len)); # endif _GL_CXXALIASWARN (getdomainname); #elif defined GNULIB_POSIXCHECK # undef getdomainname # if HAVE_RAW_DECL_GETDOMAINNAME _GL_WARN_ON_USE (getdomainname, "getdomainname is unportable - " "use gnulib module getdomainname for portability"); # endif #endif #if @GNULIB_GETDTABLESIZE@ /* Return the maximum number of file descriptors in the current process. In POSIX, this is same as sysconf (_SC_OPEN_MAX). */ # if @REPLACE_GETDTABLESIZE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getdtablesize # define getdtablesize rpl_getdtablesize # endif _GL_FUNCDECL_RPL (getdtablesize, int, (void)); _GL_CXXALIAS_RPL (getdtablesize, int, (void)); # else # if !@HAVE_GETDTABLESIZE@ _GL_FUNCDECL_SYS (getdtablesize, int, (void)); # endif _GL_CXXALIAS_SYS (getdtablesize, int, (void)); # endif _GL_CXXALIASWARN (getdtablesize); #elif defined GNULIB_POSIXCHECK # undef getdtablesize # if HAVE_RAW_DECL_GETDTABLESIZE _GL_WARN_ON_USE (getdtablesize, "getdtablesize is unportable - " "use gnulib module getdtablesize for portability"); # endif #endif #if @GNULIB_GETGROUPS@ /* Return the supplemental groups that the current process belongs to. It is unspecified whether the effective group id is in the list. If N is 0, return the group count; otherwise, N describes how many entries are available in GROUPS. Return -1 and set errno if N is not 0 and not large enough. Fails with ENOSYS on some systems. */ # if @REPLACE_GETGROUPS@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getgroups # define getgroups rpl_getgroups # endif _GL_FUNCDECL_RPL (getgroups, int, (int n, gid_t *groups)); _GL_CXXALIAS_RPL (getgroups, int, (int n, gid_t *groups)); # else # if !@HAVE_GETGROUPS@ _GL_FUNCDECL_SYS (getgroups, int, (int n, gid_t *groups)); # endif _GL_CXXALIAS_SYS (getgroups, int, (int n, gid_t *groups)); # endif _GL_CXXALIASWARN (getgroups); #elif defined GNULIB_POSIXCHECK # undef getgroups # if HAVE_RAW_DECL_GETGROUPS _GL_WARN_ON_USE (getgroups, "getgroups is unportable - " "use gnulib module getgroups for portability"); # endif #endif #if @GNULIB_GETHOSTNAME@ /* Return the standard host name of the machine. WARNING! The host name may or may not be fully qualified. Put up to LEN bytes of the host name into NAME. Null terminate it if the name is shorter than LEN. If the host name is longer than LEN, set errno = EINVAL and return -1. Return 0 if successful, otherwise set errno and return -1. */ # if @UNISTD_H_HAVE_WINSOCK2_H@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef gethostname # define gethostname rpl_gethostname # endif _GL_FUNCDECL_RPL (gethostname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (gethostname, int, (char *name, size_t len)); # else # if !@HAVE_GETHOSTNAME@ _GL_FUNCDECL_SYS (gethostname, int, (char *name, size_t len) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on Solaris 10 and OSF/1 5.1 systems, the second parameter is int len. */ _GL_CXXALIAS_SYS_CAST (gethostname, int, (char *name, size_t len)); # endif _GL_CXXALIASWARN (gethostname); #elif @UNISTD_H_HAVE_WINSOCK2_H@ # undef gethostname # define gethostname gethostname_used_without_requesting_gnulib_module_gethostname #elif defined GNULIB_POSIXCHECK # undef gethostname # if HAVE_RAW_DECL_GETHOSTNAME _GL_WARN_ON_USE (gethostname, "gethostname is unportable - " "use gnulib module gethostname for portability"); # endif #endif #if @GNULIB_GETLOGIN@ /* Returns the user's login name, or NULL if it cannot be found. Upon error, returns NULL with errno set. See . Most programs don't need to use this function, because the information is available through environment variables: ${LOGNAME-$USER} on Unix platforms, $USERNAME on native Windows platforms. */ # if !@HAVE_DECL_GETLOGIN@ _GL_FUNCDECL_SYS (getlogin, char *, (void)); # endif _GL_CXXALIAS_SYS (getlogin, char *, (void)); _GL_CXXALIASWARN (getlogin); #elif defined GNULIB_POSIXCHECK # undef getlogin # if HAVE_RAW_DECL_GETLOGIN _GL_WARN_ON_USE (getlogin, "getlogin is unportable - " "use gnulib module getlogin for portability"); # endif #endif #if @GNULIB_GETLOGIN_R@ /* Copies the user's login name to NAME. The array pointed to by NAME has room for SIZE bytes. Returns 0 if successful. Upon error, an error number is returned, or -1 in the case that the login name cannot be found but no specific error is provided (this case is hopefully rare but is left open by the POSIX spec). See . Most programs don't need to use this function, because the information is available through environment variables: ${LOGNAME-$USER} on Unix platforms, $USERNAME on native Windows platforms. */ # if @REPLACE_GETLOGIN_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getlogin_r rpl_getlogin_r # endif _GL_FUNCDECL_RPL (getlogin_r, int, (char *name, size_t size) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (getlogin_r, int, (char *name, size_t size)); # else # if !@HAVE_DECL_GETLOGIN_R@ _GL_FUNCDECL_SYS (getlogin_r, int, (char *name, size_t size) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on Solaris 10 systems, the second argument is int size. */ _GL_CXXALIAS_SYS_CAST (getlogin_r, int, (char *name, size_t size)); # endif _GL_CXXALIASWARN (getlogin_r); #elif defined GNULIB_POSIXCHECK # undef getlogin_r # if HAVE_RAW_DECL_GETLOGIN_R _GL_WARN_ON_USE (getlogin_r, "getlogin_r is unportable - " "use gnulib module getlogin_r for portability"); # endif #endif #if @GNULIB_GETPAGESIZE@ # if @REPLACE_GETPAGESIZE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getpagesize rpl_getpagesize # endif _GL_FUNCDECL_RPL (getpagesize, int, (void)); _GL_CXXALIAS_RPL (getpagesize, int, (void)); # else # if !@HAVE_GETPAGESIZE@ # if !defined getpagesize /* This is for POSIX systems. */ # if !defined _gl_getpagesize && defined _SC_PAGESIZE # if ! (defined __VMS && __VMS_VER < 70000000) # define _gl_getpagesize() sysconf (_SC_PAGESIZE) # endif # endif /* This is for older VMS. */ # if !defined _gl_getpagesize && defined __VMS # ifdef __ALPHA # define _gl_getpagesize() 8192 # else # define _gl_getpagesize() 512 # endif # endif /* This is for BeOS. */ # if !defined _gl_getpagesize && @HAVE_OS_H@ # include # if defined B_PAGE_SIZE # define _gl_getpagesize() B_PAGE_SIZE # endif # endif /* This is for AmigaOS4.0. */ # if !defined _gl_getpagesize && defined __amigaos4__ # define _gl_getpagesize() 2048 # endif /* This is for older Unix systems. */ # if !defined _gl_getpagesize && @HAVE_SYS_PARAM_H@ # include # ifdef EXEC_PAGESIZE # define _gl_getpagesize() EXEC_PAGESIZE # else # ifdef NBPG # ifndef CLSIZE # define CLSIZE 1 # endif # define _gl_getpagesize() (NBPG * CLSIZE) # else # ifdef NBPC # define _gl_getpagesize() NBPC # endif # endif # endif # endif # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define getpagesize() _gl_getpagesize () # else # if !GNULIB_defined_getpagesize_function _GL_UNISTD_INLINE int getpagesize () { return _gl_getpagesize (); } # define GNULIB_defined_getpagesize_function 1 # endif # endif # endif # endif /* Need to cast, because on Cygwin 1.5.x systems, the return type is size_t. */ _GL_CXXALIAS_SYS_CAST (getpagesize, int, (void)); # endif # if @HAVE_DECL_GETPAGESIZE@ _GL_CXXALIASWARN (getpagesize); # endif #elif defined GNULIB_POSIXCHECK # undef getpagesize # if HAVE_RAW_DECL_GETPAGESIZE _GL_WARN_ON_USE (getpagesize, "getpagesize is unportable - " "use gnulib module getpagesize for portability"); # endif #endif #if @GNULIB_GETUSERSHELL@ /* Return the next valid login shell on the system, or NULL when the end of the list has been reached. */ # if !@HAVE_DECL_GETUSERSHELL@ _GL_FUNCDECL_SYS (getusershell, char *, (void)); # endif _GL_CXXALIAS_SYS (getusershell, char *, (void)); _GL_CXXALIASWARN (getusershell); #elif defined GNULIB_POSIXCHECK # undef getusershell # if HAVE_RAW_DECL_GETUSERSHELL _GL_WARN_ON_USE (getusershell, "getusershell is unportable - " "use gnulib module getusershell for portability"); # endif #endif #if @GNULIB_GETUSERSHELL@ /* Rewind to pointer that is advanced at each getusershell() call. */ # if !@HAVE_DECL_GETUSERSHELL@ _GL_FUNCDECL_SYS (setusershell, void, (void)); # endif _GL_CXXALIAS_SYS (setusershell, void, (void)); _GL_CXXALIASWARN (setusershell); #elif defined GNULIB_POSIXCHECK # undef setusershell # if HAVE_RAW_DECL_SETUSERSHELL _GL_WARN_ON_USE (setusershell, "setusershell is unportable - " "use gnulib module getusershell for portability"); # endif #endif #if @GNULIB_GETUSERSHELL@ /* Free the pointer that is advanced at each getusershell() call and associated resources. */ # if !@HAVE_DECL_GETUSERSHELL@ _GL_FUNCDECL_SYS (endusershell, void, (void)); # endif _GL_CXXALIAS_SYS (endusershell, void, (void)); _GL_CXXALIASWARN (endusershell); #elif defined GNULIB_POSIXCHECK # undef endusershell # if HAVE_RAW_DECL_ENDUSERSHELL _GL_WARN_ON_USE (endusershell, "endusershell is unportable - " "use gnulib module getusershell for portability"); # endif #endif #if @GNULIB_GROUP_MEMBER@ /* Determine whether group id is in calling user's group list. */ # if !@HAVE_GROUP_MEMBER@ _GL_FUNCDECL_SYS (group_member, int, (gid_t gid)); # endif _GL_CXXALIAS_SYS (group_member, int, (gid_t gid)); _GL_CXXALIASWARN (group_member); #elif defined GNULIB_POSIXCHECK # undef group_member # if HAVE_RAW_DECL_GROUP_MEMBER _GL_WARN_ON_USE (group_member, "group_member is unportable - " "use gnulib module group-member for portability"); # endif #endif #if @GNULIB_ISATTY@ # if @REPLACE_ISATTY@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef isatty # define isatty rpl_isatty # endif _GL_FUNCDECL_RPL (isatty, int, (int fd)); _GL_CXXALIAS_RPL (isatty, int, (int fd)); # else _GL_CXXALIAS_SYS (isatty, int, (int fd)); # endif _GL_CXXALIASWARN (isatty); #elif defined GNULIB_POSIXCHECK # undef isatty # if HAVE_RAW_DECL_ISATTY _GL_WARN_ON_USE (isatty, "isatty has portability problems on native Windows - " "use gnulib module isatty for portability"); # endif #endif #if @GNULIB_LCHOWN@ /* Change the owner of FILE to UID (if UID is not -1) and the group of FILE to GID (if GID is not -1). Do not follow symbolic links. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_LCHOWN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef lchown # define lchown rpl_lchown # endif _GL_FUNCDECL_RPL (lchown, int, (char const *file, uid_t owner, gid_t group) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (lchown, int, (char const *file, uid_t owner, gid_t group)); # else # if !@HAVE_LCHOWN@ _GL_FUNCDECL_SYS (lchown, int, (char const *file, uid_t owner, gid_t group) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (lchown, int, (char const *file, uid_t owner, gid_t group)); # endif _GL_CXXALIASWARN (lchown); #elif defined GNULIB_POSIXCHECK # undef lchown # if HAVE_RAW_DECL_LCHOWN _GL_WARN_ON_USE (lchown, "lchown is unportable to pre-POSIX.1-2001 systems - " "use gnulib module lchown for portability"); # endif #endif #if @GNULIB_LINK@ /* Create a new hard link for an existing file. Return 0 if successful, otherwise -1 and errno set. See POSIX:2008 specification . */ # if @REPLACE_LINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define link rpl_link # endif _GL_FUNCDECL_RPL (link, int, (const char *path1, const char *path2) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (link, int, (const char *path1, const char *path2)); # else # if !@HAVE_LINK@ _GL_FUNCDECL_SYS (link, int, (const char *path1, const char *path2) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (link, int, (const char *path1, const char *path2)); # endif _GL_CXXALIASWARN (link); #elif defined GNULIB_POSIXCHECK # undef link # if HAVE_RAW_DECL_LINK _GL_WARN_ON_USE (link, "link is unportable - " "use gnulib module link for portability"); # endif #endif #if @GNULIB_LINKAT@ /* Create a new hard link for an existing file, relative to two directories. FLAG controls whether symlinks are followed. Return 0 if successful, otherwise -1 and errno set. */ # if @REPLACE_LINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef linkat # define linkat rpl_linkat # endif _GL_FUNCDECL_RPL (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag) _GL_ARG_NONNULL ((2, 4))); _GL_CXXALIAS_RPL (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag)); # else # if !@HAVE_LINKAT@ _GL_FUNCDECL_SYS (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag) _GL_ARG_NONNULL ((2, 4))); # endif _GL_CXXALIAS_SYS (linkat, int, (int fd1, const char *path1, int fd2, const char *path2, int flag)); # endif _GL_CXXALIASWARN (linkat); #elif defined GNULIB_POSIXCHECK # undef linkat # if HAVE_RAW_DECL_LINKAT _GL_WARN_ON_USE (linkat, "linkat is unportable - " "use gnulib module linkat for portability"); # endif #endif #if @GNULIB_LSEEK@ /* Set the offset of FD relative to SEEK_SET, SEEK_CUR, or SEEK_END. Return the new offset if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_LSEEK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define lseek rpl_lseek # endif _GL_FUNCDECL_RPL (lseek, off_t, (int fd, off_t offset, int whence)); _GL_CXXALIAS_RPL (lseek, off_t, (int fd, off_t offset, int whence)); # else _GL_CXXALIAS_SYS (lseek, off_t, (int fd, off_t offset, int whence)); # endif _GL_CXXALIASWARN (lseek); #elif defined GNULIB_POSIXCHECK # undef lseek # if HAVE_RAW_DECL_LSEEK _GL_WARN_ON_USE (lseek, "lseek does not fail with ESPIPE on pipes on some " "systems - use gnulib module lseek for portability"); # endif #endif #if @GNULIB_PIPE@ /* Create a pipe, defaulting to O_BINARY mode. Store the read-end as fd[0] and the write-end as fd[1]. Return 0 upon success, or -1 with errno set upon failure. */ # if !@HAVE_PIPE@ _GL_FUNCDECL_SYS (pipe, int, (int fd[2]) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (pipe, int, (int fd[2])); _GL_CXXALIASWARN (pipe); #elif defined GNULIB_POSIXCHECK # undef pipe # if HAVE_RAW_DECL_PIPE _GL_WARN_ON_USE (pipe, "pipe is unportable - " "use gnulib module pipe-posix for portability"); # endif #endif #if @GNULIB_PIPE2@ /* Create a pipe, applying the given flags when opening the read-end of the pipe and the write-end of the pipe. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). Store the read-end as fd[0] and the write-end as fd[1]. Return 0 upon success, or -1 with errno set upon failure. See also the Linux man page at . */ # if @HAVE_PIPE2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define pipe2 rpl_pipe2 # endif _GL_FUNCDECL_RPL (pipe2, int, (int fd[2], int flags) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (pipe2, int, (int fd[2], int flags)); # else _GL_FUNCDECL_SYS (pipe2, int, (int fd[2], int flags) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (pipe2, int, (int fd[2], int flags)); # endif _GL_CXXALIASWARN (pipe2); #elif defined GNULIB_POSIXCHECK # undef pipe2 # if HAVE_RAW_DECL_PIPE2 _GL_WARN_ON_USE (pipe2, "pipe2 is unportable - " "use gnulib module pipe2 for portability"); # endif #endif #if @GNULIB_PREAD@ /* Read at most BUFSIZE bytes from FD into BUF, starting at OFFSET. Return the number of bytes placed into BUF if successful, otherwise set errno and return -1. 0 indicates EOF. See the POSIX:2008 specification . */ # if @REPLACE_PREAD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef pread # define pread rpl_pread # endif _GL_FUNCDECL_RPL (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset)); # else # if !@HAVE_PREAD@ _GL_FUNCDECL_SYS (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (pread, ssize_t, (int fd, void *buf, size_t bufsize, off_t offset)); # endif _GL_CXXALIASWARN (pread); #elif defined GNULIB_POSIXCHECK # undef pread # if HAVE_RAW_DECL_PREAD _GL_WARN_ON_USE (pread, "pread is unportable - " "use gnulib module pread for portability"); # endif #endif #if @GNULIB_PWRITE@ /* Write at most BUFSIZE bytes from BUF into FD, starting at OFFSET. Return the number of bytes written if successful, otherwise set errno and return -1. 0 indicates nothing written. See the POSIX:2008 specification . */ # if @REPLACE_PWRITE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef pwrite # define pwrite rpl_pwrite # endif _GL_FUNCDECL_RPL (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset)); # else # if !@HAVE_PWRITE@ _GL_FUNCDECL_SYS (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (pwrite, ssize_t, (int fd, const void *buf, size_t bufsize, off_t offset)); # endif _GL_CXXALIASWARN (pwrite); #elif defined GNULIB_POSIXCHECK # undef pwrite # if HAVE_RAW_DECL_PWRITE _GL_WARN_ON_USE (pwrite, "pwrite is unportable - " "use gnulib module pwrite for portability"); # endif #endif #if @GNULIB_READ@ /* Read up to COUNT bytes from file descriptor FD into the buffer starting at BUF. See the POSIX:2008 specification . */ # if @REPLACE_READ@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef read # define read rpl_read # endif _GL_FUNCDECL_RPL (read, ssize_t, (int fd, void *buf, size_t count) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (read, ssize_t, (int fd, void *buf, size_t count)); # else /* Need to cast, because on mingw, the third parameter is unsigned int count and the return type is 'int'. */ _GL_CXXALIAS_SYS_CAST (read, ssize_t, (int fd, void *buf, size_t count)); # endif _GL_CXXALIASWARN (read); #endif #if @GNULIB_READLINK@ /* Read the contents of the symbolic link FILE and place the first BUFSIZE bytes of it into BUF. Return the number of bytes placed into BUF if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_READLINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define readlink rpl_readlink # endif _GL_FUNCDECL_RPL (readlink, ssize_t, (const char *file, char *buf, size_t bufsize) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (readlink, ssize_t, (const char *file, char *buf, size_t bufsize)); # else # if !@HAVE_READLINK@ _GL_FUNCDECL_SYS (readlink, ssize_t, (const char *file, char *buf, size_t bufsize) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (readlink, ssize_t, (const char *file, char *buf, size_t bufsize)); # endif _GL_CXXALIASWARN (readlink); #elif defined GNULIB_POSIXCHECK # undef readlink # if HAVE_RAW_DECL_READLINK _GL_WARN_ON_USE (readlink, "readlink is unportable - " "use gnulib module readlink for portability"); # endif #endif #if @GNULIB_READLINKAT@ # if @REPLACE_READLINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define readlinkat rpl_readlinkat # endif _GL_FUNCDECL_RPL (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len)); # else # if !@HAVE_READLINKAT@ _GL_FUNCDECL_SYS (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (readlinkat, ssize_t, (int fd, char const *file, char *buf, size_t len)); # endif _GL_CXXALIASWARN (readlinkat); #elif defined GNULIB_POSIXCHECK # undef readlinkat # if HAVE_RAW_DECL_READLINKAT _GL_WARN_ON_USE (readlinkat, "readlinkat is not portable - " "use gnulib module readlinkat for portability"); # endif #endif #if @GNULIB_RMDIR@ /* Remove the directory DIR. */ # if @REPLACE_RMDIR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define rmdir rpl_rmdir # endif _GL_FUNCDECL_RPL (rmdir, int, (char const *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (rmdir, int, (char const *name)); # else _GL_CXXALIAS_SYS (rmdir, int, (char const *name)); # endif _GL_CXXALIASWARN (rmdir); #elif defined GNULIB_POSIXCHECK # undef rmdir # if HAVE_RAW_DECL_RMDIR _GL_WARN_ON_USE (rmdir, "rmdir is unportable - " "use gnulib module rmdir for portability"); # endif #endif #if @GNULIB_SETHOSTNAME@ /* Set the host name of the machine. The host name may or may not be fully qualified. Put LEN bytes of NAME into the host name. Return 0 if successful, otherwise, set errno and return -1. Platforms with no ability to set the hostname return -1 and set errno = ENOSYS. */ # if !@HAVE_SETHOSTNAME@ || !@HAVE_DECL_SETHOSTNAME@ _GL_FUNCDECL_SYS (sethostname, int, (const char *name, size_t len) _GL_ARG_NONNULL ((1))); # endif /* Need to cast, because on Solaris 11 2011-10, Mac OS X 10.5, IRIX 6.5 and FreeBSD 6.4 the second parameter is int. On Solaris 11 2011-10, the first parameter is not const. */ _GL_CXXALIAS_SYS_CAST (sethostname, int, (const char *name, size_t len)); _GL_CXXALIASWARN (sethostname); #elif defined GNULIB_POSIXCHECK # undef sethostname # if HAVE_RAW_DECL_SETHOSTNAME _GL_WARN_ON_USE (sethostname, "sethostname is unportable - " "use gnulib module sethostname for portability"); # endif #endif #if @GNULIB_SLEEP@ /* Pause the execution of the current thread for N seconds. Returns the number of seconds left to sleep. See the POSIX:2008 specification . */ # if @REPLACE_SLEEP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sleep # define sleep rpl_sleep # endif _GL_FUNCDECL_RPL (sleep, unsigned int, (unsigned int n)); _GL_CXXALIAS_RPL (sleep, unsigned int, (unsigned int n)); # else # if !@HAVE_SLEEP@ _GL_FUNCDECL_SYS (sleep, unsigned int, (unsigned int n)); # endif _GL_CXXALIAS_SYS (sleep, unsigned int, (unsigned int n)); # endif _GL_CXXALIASWARN (sleep); #elif defined GNULIB_POSIXCHECK # undef sleep # if HAVE_RAW_DECL_SLEEP _GL_WARN_ON_USE (sleep, "sleep is unportable - " "use gnulib module sleep for portability"); # endif #endif #if @GNULIB_SYMLINK@ # if @REPLACE_SYMLINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef symlink # define symlink rpl_symlink # endif _GL_FUNCDECL_RPL (symlink, int, (char const *contents, char const *file) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (symlink, int, (char const *contents, char const *file)); # else # if !@HAVE_SYMLINK@ _GL_FUNCDECL_SYS (symlink, int, (char const *contents, char const *file) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (symlink, int, (char const *contents, char const *file)); # endif _GL_CXXALIASWARN (symlink); #elif defined GNULIB_POSIXCHECK # undef symlink # if HAVE_RAW_DECL_SYMLINK _GL_WARN_ON_USE (symlink, "symlink is not portable - " "use gnulib module symlink for portability"); # endif #endif #if @GNULIB_SYMLINKAT@ # if @REPLACE_SYMLINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef symlinkat # define symlinkat rpl_symlinkat # endif _GL_FUNCDECL_RPL (symlinkat, int, (char const *contents, int fd, char const *file) _GL_ARG_NONNULL ((1, 3))); _GL_CXXALIAS_RPL (symlinkat, int, (char const *contents, int fd, char const *file)); # else # if !@HAVE_SYMLINKAT@ _GL_FUNCDECL_SYS (symlinkat, int, (char const *contents, int fd, char const *file) _GL_ARG_NONNULL ((1, 3))); # endif _GL_CXXALIAS_SYS (symlinkat, int, (char const *contents, int fd, char const *file)); # endif _GL_CXXALIASWARN (symlinkat); #elif defined GNULIB_POSIXCHECK # undef symlinkat # if HAVE_RAW_DECL_SYMLINKAT _GL_WARN_ON_USE (symlinkat, "symlinkat is not portable - " "use gnulib module symlinkat for portability"); # endif #endif #if @GNULIB_TRUNCATE@ /* Change the size of the file designated by FILENAME to become equal to LENGTH. Return 0 if successful, otherwise -1 and errno set. See the POSIX:2008 specification . */ # if @REPLACE_TRUNCATE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef truncate # define truncate rpl_truncate # endif _GL_FUNCDECL_RPL (truncate, int, (const char *filename, off_t length) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (truncate, int, (const char *filename, off_t length)); # else # if !@HAVE_TRUNCATE@ _GL_FUNCDECL_SYS (truncate, int, (const char *filename, off_t length) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (truncate, int, (const char *filename, off_t length)); # endif _GL_CXXALIASWARN (truncate); #elif defined GNULIB_POSIXCHECK # undef truncate # if HAVE_RAW_DECL_TRUNCATE _GL_WARN_ON_USE (truncate, "truncate is unportable - " "use gnulib module truncate for portability"); # endif #endif #if @GNULIB_TTYNAME_R@ /* Store at most BUFLEN characters of the pathname of the terminal FD is open on in BUF. Return 0 on success, otherwise an error number. */ # if @REPLACE_TTYNAME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ttyname_r # define ttyname_r rpl_ttyname_r # endif _GL_FUNCDECL_RPL (ttyname_r, int, (int fd, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (ttyname_r, int, (int fd, char *buf, size_t buflen)); # else # if !@HAVE_DECL_TTYNAME_R@ _GL_FUNCDECL_SYS (ttyname_r, int, (int fd, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (ttyname_r, int, (int fd, char *buf, size_t buflen)); # endif _GL_CXXALIASWARN (ttyname_r); #elif defined GNULIB_POSIXCHECK # undef ttyname_r # if HAVE_RAW_DECL_TTYNAME_R _GL_WARN_ON_USE (ttyname_r, "ttyname_r is not portable - " "use gnulib module ttyname_r for portability"); # endif #endif #if @GNULIB_UNLINK@ # if @REPLACE_UNLINK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef unlink # define unlink rpl_unlink # endif _GL_FUNCDECL_RPL (unlink, int, (char const *file) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (unlink, int, (char const *file)); # else _GL_CXXALIAS_SYS (unlink, int, (char const *file)); # endif _GL_CXXALIASWARN (unlink); #elif defined GNULIB_POSIXCHECK # undef unlink # if HAVE_RAW_DECL_UNLINK _GL_WARN_ON_USE (unlink, "unlink is not portable - " "use gnulib module unlink for portability"); # endif #endif #if @GNULIB_UNLINKAT@ # if @REPLACE_UNLINKAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef unlinkat # define unlinkat rpl_unlinkat # endif _GL_FUNCDECL_RPL (unlinkat, int, (int fd, char const *file, int flag) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (unlinkat, int, (int fd, char const *file, int flag)); # else # if !@HAVE_UNLINKAT@ _GL_FUNCDECL_SYS (unlinkat, int, (int fd, char const *file, int flag) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (unlinkat, int, (int fd, char const *file, int flag)); # endif _GL_CXXALIASWARN (unlinkat); #elif defined GNULIB_POSIXCHECK # undef unlinkat # if HAVE_RAW_DECL_UNLINKAT _GL_WARN_ON_USE (unlinkat, "unlinkat is not portable - " "use gnulib module openat for portability"); # endif #endif #if @GNULIB_USLEEP@ /* Pause the execution of the current thread for N microseconds. Returns 0 on completion, or -1 on range error. See the POSIX:2001 specification . */ # if @REPLACE_USLEEP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef usleep # define usleep rpl_usleep # endif _GL_FUNCDECL_RPL (usleep, int, (useconds_t n)); _GL_CXXALIAS_RPL (usleep, int, (useconds_t n)); # else # if !@HAVE_USLEEP@ _GL_FUNCDECL_SYS (usleep, int, (useconds_t n)); # endif _GL_CXXALIAS_SYS (usleep, int, (useconds_t n)); # endif _GL_CXXALIASWARN (usleep); #elif defined GNULIB_POSIXCHECK # undef usleep # if HAVE_RAW_DECL_USLEEP _GL_WARN_ON_USE (usleep, "usleep is unportable - " "use gnulib module usleep for portability"); # endif #endif #if @GNULIB_WRITE@ /* Write up to COUNT bytes starting at BUF to file descriptor FD. See the POSIX:2008 specification . */ # if @REPLACE_WRITE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef write # define write rpl_write # endif _GL_FUNCDECL_RPL (write, ssize_t, (int fd, const void *buf, size_t count) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (write, ssize_t, (int fd, const void *buf, size_t count)); # else /* Need to cast, because on mingw, the third parameter is unsigned int count and the return type is 'int'. */ _GL_CXXALIAS_SYS_CAST (write, ssize_t, (int fd, const void *buf, size_t count)); # endif _GL_CXXALIASWARN (write); #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_UNISTD_H */ #endif /* _GL_INCLUDING_UNISTD_H */ #endif /* _@GUARD_PREFIX@_UNISTD_H */ gnuastro-0.5/bootstrapped/lib/sysexits.in.h0000644000175000017500000000365613217200021016064 00000000000000/* exit() exit codes for some BSD system programs. Copyright (C) 2003, 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Simon Josefsson based on sysexits(3) man page */ #ifndef _@GUARD_PREFIX@_SYSEXITS_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if @HAVE_SYSEXITS_H@ /* IRIX 6.5 has an that defines a macro EX_OK with a nonzero value. Override it. See */ # ifdef __sgi # include # undef EX_OK # endif /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_SYSEXITS_H@ /* HP-UX 11 ends at EX_NOPERM. */ # ifndef EX_CONFIG # define EX_CONFIG 78 # endif #endif #ifndef _@GUARD_PREFIX@_SYSEXITS_H #define _@GUARD_PREFIX@_SYSEXITS_H #if !@HAVE_SYSEXITS_H@ # define EX_OK 0 /* same value as EXIT_SUCCESS */ # define EX_USAGE 64 # define EX_DATAERR 65 # define EX_NOINPUT 66 # define EX_NOUSER 67 # define EX_NOHOST 68 # define EX_UNAVAILABLE 69 # define EX_SOFTWARE 70 # define EX_OSERR 71 # define EX_OSFILE 72 # define EX_CANTCREAT 73 # define EX_IOERR 74 # define EX_TEMPFAIL 75 # define EX_PROTOCOL 76 # define EX_NOPERM 77 # define EX_CONFIG 78 #endif #endif /* _@GUARD_PREFIX@_SYSEXITS_H */ #endif /* _@GUARD_PREFIX@_SYSEXITS_H */ gnuastro-0.5/bootstrapped/lib/sys_types.in.h0000644000175000017500000000545013217200021016225 00000000000000/* Provide a more complete sys/types.h. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #ifndef _@GUARD_PREFIX@_SYS_TYPES_H /* The include_next requires a split double-inclusion guard. */ # define _GL_INCLUDING_SYS_TYPES_H #@INCLUDE_NEXT@ @NEXT_SYS_TYPES_H@ # undef _GL_INCLUDING_SYS_TYPES_H #ifndef _@GUARD_PREFIX@_SYS_TYPES_H #define _@GUARD_PREFIX@_SYS_TYPES_H /* Override off_t if Large File Support is requested on native Windows. */ #if @WINDOWS_64_BIT_OFF_T@ /* Same as int64_t in . */ # if defined _MSC_VER # define off_t __int64 # else # define off_t long long int # endif /* Indicator, for gnulib internal purposes. */ # define _GL_WINDOWS_64_BIT_OFF_T 1 #endif /* Override dev_t and ino_t if distinguishable inodes support is requested on native Windows. */ #if @WINDOWS_STAT_INODES@ # if @WINDOWS_STAT_INODES@ == 2 /* Experimental, not useful in Windows 10. */ /* Define dev_t to a 64-bit type. */ # if !defined GNULIB_defined_dev_t typedef unsigned long long int rpl_dev_t; # undef dev_t # define dev_t rpl_dev_t # define GNULIB_defined_dev_t 1 # endif /* Define ino_t to a 128-bit type. */ # if !defined GNULIB_defined_ino_t /* MSVC does not have a 128-bit integer type. GCC has a 128-bit integer type __int128, but only on 64-bit targets. */ typedef struct { unsigned long long int _gl_ino[2]; } rpl_ino_t; # undef ino_t # define ino_t rpl_ino_t # define GNULIB_defined_ino_t 1 # endif # else /* @WINDOWS_STAT_INODES@ == 1 */ /* Define ino_t to a 64-bit type. */ # if !defined GNULIB_defined_ino_t typedef unsigned long long int rpl_ino_t; # undef ino_t # define ino_t rpl_ino_t # define GNULIB_defined_ino_t 1 # endif # endif /* Indicator, for gnulib internal purposes. */ # define _GL_WINDOWS_STAT_INODES @WINDOWS_STAT_INODES@ #endif /* MSVC 9 defines size_t in , not in . */ /* But avoid namespace pollution on glibc systems. */ #if ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) \ && ! defined __GLIBC__ # include #endif #endif /* _@GUARD_PREFIX@_SYS_TYPES_H */ #endif /* _@GUARD_PREFIX@_SYS_TYPES_H */ gnuastro-0.5/bootstrapped/lib/strings.in.h0000644000175000017500000000765713217200021015667 00000000000000/* A substitute . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_STRINGS_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Minix 3.1.8 has a bug: must be included before . But avoid namespace pollution on glibc systems. */ #if defined __minix && !defined __GLIBC__ # include #endif /* The include_next requires a split double-inclusion guard. */ #if @HAVE_STRINGS_H@ # @INCLUDE_NEXT@ @NEXT_STRINGS_H@ #endif #ifndef _@GUARD_PREFIX@_STRINGS_H #define _@GUARD_PREFIX@_STRINGS_H #if ! @HAVE_DECL_STRNCASECMP@ /* Get size_t. */ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #ifdef __cplusplus extern "C" { #endif /* Find the index of the least-significant set bit. */ #if @GNULIB_FFS@ # if !@HAVE_FFS@ _GL_FUNCDECL_SYS (ffs, int, (int i)); # endif _GL_CXXALIAS_SYS (ffs, int, (int i)); _GL_CXXALIASWARN (ffs); #elif defined GNULIB_POSIXCHECK # undef ffs # if HAVE_RAW_DECL_FFS _GL_WARN_ON_USE (ffs, "ffs is not portable - use the ffs module"); # endif #endif /* Compare strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function does not work in multibyte locales. */ #if ! @HAVE_STRCASECMP@ extern int strcasecmp (char const *s1, char const *s2) _GL_ARG_NONNULL ((1, 2)); #endif #if defined GNULIB_POSIXCHECK /* strcasecmp() does not work with multibyte strings: POSIX says that it operates on "strings", and "string" in POSIX is defined as a sequence of bytes, not of characters. */ # undef strcasecmp # if HAVE_RAW_DECL_STRCASECMP _GL_WARN_ON_USE (strcasecmp, "strcasecmp cannot work correctly on character " "strings in multibyte locales - " "use mbscasecmp if you care about " "internationalization, or use c_strcasecmp , " "gnulib module c-strcase) if you want a locale " "independent function"); # endif #endif /* Compare no more than N bytes of strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function cannot work correctly in multibyte locales. */ #if ! @HAVE_DECL_STRNCASECMP@ extern int strncasecmp (char const *s1, char const *s2, size_t n) _GL_ARG_NONNULL ((1, 2)); #endif #if defined GNULIB_POSIXCHECK /* strncasecmp() does not work with multibyte strings: POSIX says that it operates on "strings", and "string" in POSIX is defined as a sequence of bytes, not of characters. */ # undef strncasecmp # if HAVE_RAW_DECL_STRNCASECMP _GL_WARN_ON_USE (strncasecmp, "strncasecmp cannot work correctly on character " "strings in multibyte locales - " "use mbsncasecmp or mbspcasecmp if you care about " "internationalization, or use c_strncasecmp , " "gnulib module c-strcase) if you want a locale " "independent function"); # endif #endif #ifdef __cplusplus } #endif #endif /* _@GUARD_PREFIX@_STRING_H */ #endif /* _@GUARD_PREFIX@_STRING_H */ gnuastro-0.5/bootstrapped/lib/string.in.h0000644000175000017500000012056113217200021015472 00000000000000/* A GNU-like . Copyright (C) 1995-1996, 2001-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined _GL_ALREADY_INCLUDING_STRING_H /* Special invocation convention: - On OS X/NetBSD we have a sequence of nested includes -> -> "string.h" In this situation system _chk variants due to -D_FORTIFY_SOURCE might be used after any replacements defined here. */ #@INCLUDE_NEXT@ @NEXT_STRING_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_STRING_H #define _GL_ALREADY_INCLUDING_STRING_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_STRING_H@ #undef _GL_ALREADY_INCLUDING_STRING_H #ifndef _@GUARD_PREFIX@_STRING_H #define _@GUARD_PREFIX@_STRING_H /* NetBSD 5.0 mis-defines NULL. */ #include /* MirBSD defines mbslen as a macro. */ #if @GNULIB_MBSLEN@ && defined __MirBSD__ # include #endif /* The __attribute__ feature is available in gcc versions 2.5 and later. The attribute __pure__ was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* NetBSD 5.0 declares strsignal in , not in . */ /* But in any case avoid namespace pollution on glibc systems. */ #if (@GNULIB_STRSIGNAL@ || defined GNULIB_POSIXCHECK) && defined __NetBSD__ \ && ! defined __GLIBC__ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Clear a block of memory. The compiler will not delete a call to this function, even if the block is dead after the call. */ #if @GNULIB_EXPLICIT_BZERO@ # if ! @HAVE_EXPLICIT_BZERO@ _GL_FUNCDECL_SYS (explicit_bzero, void, (void *__dest, size_t __n) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (explicit_bzero, void, (void *__dest, size_t __n)); _GL_CXXALIASWARN (explicit_bzero); #elif defined GNULIB_POSIXCHECK # undef explicit_bzero # if HAVE_RAW_DECL_EXPLICIT_BZERO _GL_WARN_ON_USE (explicit_bzero, "explicit_bzero is unportable - " "use gnulib module explicit_bzero for portability"); # endif #endif /* Find the index of the least-significant set bit. */ #if @GNULIB_FFSL@ # if !@HAVE_FFSL@ _GL_FUNCDECL_SYS (ffsl, int, (long int i)); # endif _GL_CXXALIAS_SYS (ffsl, int, (long int i)); _GL_CXXALIASWARN (ffsl); #elif defined GNULIB_POSIXCHECK # undef ffsl # if HAVE_RAW_DECL_FFSL _GL_WARN_ON_USE (ffsl, "ffsl is not portable - use the ffsl module"); # endif #endif /* Find the index of the least-significant set bit. */ #if @GNULIB_FFSLL@ # if !@HAVE_FFSLL@ _GL_FUNCDECL_SYS (ffsll, int, (long long int i)); # endif _GL_CXXALIAS_SYS (ffsll, int, (long long int i)); _GL_CXXALIASWARN (ffsll); #elif defined GNULIB_POSIXCHECK # undef ffsll # if HAVE_RAW_DECL_FFSLL _GL_WARN_ON_USE (ffsll, "ffsll is not portable - use the ffsll module"); # endif #endif /* Return the first instance of C within N bytes of S, or NULL. */ #if @GNULIB_MEMCHR@ # if @REPLACE_MEMCHR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define memchr rpl_memchr # endif _GL_FUNCDECL_RPL (memchr, void *, (void const *__s, int __c, size_t __n) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (memchr, void *, (void const *__s, int __c, size_t __n)); # else # if ! @HAVE_MEMCHR@ _GL_FUNCDECL_SYS (memchr, void *, (void const *__s, int __c, size_t __n) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C" { const void * std::memchr (const void *, int, size_t); } extern "C++" { void * std::memchr (void *, int, size_t); } */ _GL_CXXALIAS_SYS_CAST2 (memchr, void *, (void const *__s, int __c, size_t __n), void const *, (void const *__s, int __c, size_t __n)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (memchr, void *, (void *__s, int __c, size_t __n)); _GL_CXXALIASWARN1 (memchr, void const *, (void const *__s, int __c, size_t __n)); # else _GL_CXXALIASWARN (memchr); # endif #elif defined GNULIB_POSIXCHECK # undef memchr /* Assume memchr is always declared. */ _GL_WARN_ON_USE (memchr, "memchr has platform-specific bugs - " "use gnulib module memchr for portability" ); #endif /* Return the first occurrence of NEEDLE in HAYSTACK. */ #if @GNULIB_MEMMEM@ # if @REPLACE_MEMMEM@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define memmem rpl_memmem # endif _GL_FUNCDECL_RPL (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 3))); _GL_CXXALIAS_RPL (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len)); # else # if ! @HAVE_DECL_MEMMEM@ _GL_FUNCDECL_SYS (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 3))); # endif _GL_CXXALIAS_SYS (memmem, void *, (void const *__haystack, size_t __haystack_len, void const *__needle, size_t __needle_len)); # endif _GL_CXXALIASWARN (memmem); #elif defined GNULIB_POSIXCHECK # undef memmem # if HAVE_RAW_DECL_MEMMEM _GL_WARN_ON_USE (memmem, "memmem is unportable and often quadratic - " "use gnulib module memmem-simple for portability, " "and module memmem for speed" ); # endif #endif /* Copy N bytes of SRC to DEST, return pointer to bytes after the last written byte. */ #if @GNULIB_MEMPCPY@ # if ! @HAVE_MEMPCPY@ _GL_FUNCDECL_SYS (mempcpy, void *, (void *restrict __dest, void const *restrict __src, size_t __n) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (mempcpy, void *, (void *restrict __dest, void const *restrict __src, size_t __n)); _GL_CXXALIASWARN (mempcpy); #elif defined GNULIB_POSIXCHECK # undef mempcpy # if HAVE_RAW_DECL_MEMPCPY _GL_WARN_ON_USE (mempcpy, "mempcpy is unportable - " "use gnulib module mempcpy for portability"); # endif #endif /* Search backwards through a block for a byte (specified as an int). */ #if @GNULIB_MEMRCHR@ # if ! @HAVE_DECL_MEMRCHR@ _GL_FUNCDECL_SYS (memrchr, void *, (void const *, int, size_t) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const void * std::memrchr (const void *, int, size_t); } extern "C++" { void * std::memrchr (void *, int, size_t); } */ _GL_CXXALIAS_SYS_CAST2 (memrchr, void *, (void const *, int, size_t), void const *, (void const *, int, size_t)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (memrchr, void *, (void *, int, size_t)); _GL_CXXALIASWARN1 (memrchr, void const *, (void const *, int, size_t)); # else _GL_CXXALIASWARN (memrchr); # endif #elif defined GNULIB_POSIXCHECK # undef memrchr # if HAVE_RAW_DECL_MEMRCHR _GL_WARN_ON_USE (memrchr, "memrchr is unportable - " "use gnulib module memrchr for portability"); # endif #endif /* Find the first occurrence of C in S. More efficient than memchr(S,C,N), at the expense of undefined behavior if C does not occur within N bytes. */ #if @GNULIB_RAWMEMCHR@ # if ! @HAVE_RAWMEMCHR@ _GL_FUNCDECL_SYS (rawmemchr, void *, (void const *__s, int __c_in) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const void * std::rawmemchr (const void *, int); } extern "C++" { void * std::rawmemchr (void *, int); } */ _GL_CXXALIAS_SYS_CAST2 (rawmemchr, void *, (void const *__s, int __c_in), void const *, (void const *__s, int __c_in)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (rawmemchr, void *, (void *__s, int __c_in)); _GL_CXXALIASWARN1 (rawmemchr, void const *, (void const *__s, int __c_in)); # else _GL_CXXALIASWARN (rawmemchr); # endif #elif defined GNULIB_POSIXCHECK # undef rawmemchr # if HAVE_RAW_DECL_RAWMEMCHR _GL_WARN_ON_USE (rawmemchr, "rawmemchr is unportable - " "use gnulib module rawmemchr for portability"); # endif #endif /* Copy SRC to DST, returning the address of the terminating '\0' in DST. */ #if @GNULIB_STPCPY@ # if ! @HAVE_STPCPY@ _GL_FUNCDECL_SYS (stpcpy, char *, (char *restrict __dst, char const *restrict __src) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (stpcpy, char *, (char *restrict __dst, char const *restrict __src)); _GL_CXXALIASWARN (stpcpy); #elif defined GNULIB_POSIXCHECK # undef stpcpy # if HAVE_RAW_DECL_STPCPY _GL_WARN_ON_USE (stpcpy, "stpcpy is unportable - " "use gnulib module stpcpy for portability"); # endif #endif /* Copy no more than N bytes of SRC to DST, returning a pointer past the last non-NUL byte written into DST. */ #if @GNULIB_STPNCPY@ # if @REPLACE_STPNCPY@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef stpncpy # define stpncpy rpl_stpncpy # endif _GL_FUNCDECL_RPL (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n)); # else # if ! @HAVE_STPNCPY@ _GL_FUNCDECL_SYS (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (stpncpy, char *, (char *restrict __dst, char const *restrict __src, size_t __n)); # endif _GL_CXXALIASWARN (stpncpy); #elif defined GNULIB_POSIXCHECK # undef stpncpy # if HAVE_RAW_DECL_STPNCPY _GL_WARN_ON_USE (stpncpy, "stpncpy is unportable - " "use gnulib module stpncpy for portability"); # endif #endif #if defined GNULIB_POSIXCHECK /* strchr() does not work with multibyte strings if the locale encoding is GB18030 and the character to be searched is a digit. */ # undef strchr /* Assume strchr is always declared. */ _GL_WARN_ON_USE (strchr, "strchr cannot work correctly on character strings " "in some multibyte locales - " "use mbschr if you care about internationalization"); #endif /* Find the first occurrence of C in S or the final NUL byte. */ #if @GNULIB_STRCHRNUL@ # if @REPLACE_STRCHRNUL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strchrnul rpl_strchrnul # endif _GL_FUNCDECL_RPL (strchrnul, char *, (const char *__s, int __c_in) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strchrnul, char *, (const char *str, int ch)); # else # if ! @HAVE_STRCHRNUL@ _GL_FUNCDECL_SYS (strchrnul, char *, (char const *__s, int __c_in) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const char * std::strchrnul (const char *, int); } extern "C++" { char * std::strchrnul (char *, int); } */ _GL_CXXALIAS_SYS_CAST2 (strchrnul, char *, (char const *__s, int __c_in), char const *, (char const *__s, int __c_in)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strchrnul, char *, (char *__s, int __c_in)); _GL_CXXALIASWARN1 (strchrnul, char const *, (char const *__s, int __c_in)); # else _GL_CXXALIASWARN (strchrnul); # endif #elif defined GNULIB_POSIXCHECK # undef strchrnul # if HAVE_RAW_DECL_STRCHRNUL _GL_WARN_ON_USE (strchrnul, "strchrnul is unportable - " "use gnulib module strchrnul for portability"); # endif #endif /* Duplicate S, returning an identical malloc'd string. */ #if @GNULIB_STRDUP@ # if @REPLACE_STRDUP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strdup # define strdup rpl_strdup # endif _GL_FUNCDECL_RPL (strdup, char *, (char const *__s) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strdup, char *, (char const *__s)); # else # if defined __cplusplus && defined GNULIB_NAMESPACE && defined strdup /* strdup exists as a function and as a macro. Get rid of the macro. */ # undef strdup # endif # if !(@HAVE_DECL_STRDUP@ || defined strdup) _GL_FUNCDECL_SYS (strdup, char *, (char const *__s) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strdup, char *, (char const *__s)); # endif _GL_CXXALIASWARN (strdup); #elif defined GNULIB_POSIXCHECK # undef strdup # if HAVE_RAW_DECL_STRDUP _GL_WARN_ON_USE (strdup, "strdup is unportable - " "use gnulib module strdup for portability"); # endif #endif /* Append no more than N characters from SRC onto DEST. */ #if @GNULIB_STRNCAT@ # if @REPLACE_STRNCAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strncat # define strncat rpl_strncat # endif _GL_FUNCDECL_RPL (strncat, char *, (char *dest, const char *src, size_t n) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (strncat, char *, (char *dest, const char *src, size_t n)); # else _GL_CXXALIAS_SYS (strncat, char *, (char *dest, const char *src, size_t n)); # endif _GL_CXXALIASWARN (strncat); #elif defined GNULIB_POSIXCHECK # undef strncat # if HAVE_RAW_DECL_STRNCAT _GL_WARN_ON_USE (strncat, "strncat is unportable - " "use gnulib module strncat for portability"); # endif #endif /* Return a newly allocated copy of at most N bytes of STRING. */ #if @GNULIB_STRNDUP@ # if @REPLACE_STRNDUP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strndup # define strndup rpl_strndup # endif _GL_FUNCDECL_RPL (strndup, char *, (char const *__s, size_t __n) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strndup, char *, (char const *__s, size_t __n)); # else # if ! @HAVE_DECL_STRNDUP@ _GL_FUNCDECL_SYS (strndup, char *, (char const *__s, size_t __n) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strndup, char *, (char const *__s, size_t __n)); # endif _GL_CXXALIASWARN (strndup); #elif defined GNULIB_POSIXCHECK # undef strndup # if HAVE_RAW_DECL_STRNDUP _GL_WARN_ON_USE (strndup, "strndup is unportable - " "use gnulib module strndup for portability"); # endif #endif /* Find the length (number of bytes) of STRING, but scan at most MAXLEN bytes. If no '\0' terminator is found in that many bytes, return MAXLEN. */ #if @GNULIB_STRNLEN@ # if @REPLACE_STRNLEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strnlen # define strnlen rpl_strnlen # endif _GL_FUNCDECL_RPL (strnlen, size_t, (char const *__s, size_t __maxlen) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strnlen, size_t, (char const *__s, size_t __maxlen)); # else # if ! @HAVE_DECL_STRNLEN@ _GL_FUNCDECL_SYS (strnlen, size_t, (char const *__s, size_t __maxlen) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strnlen, size_t, (char const *__s, size_t __maxlen)); # endif _GL_CXXALIASWARN (strnlen); #elif defined GNULIB_POSIXCHECK # undef strnlen # if HAVE_RAW_DECL_STRNLEN _GL_WARN_ON_USE (strnlen, "strnlen is unportable - " "use gnulib module strnlen for portability"); # endif #endif #if defined GNULIB_POSIXCHECK /* strcspn() assumes the second argument is a list of single-byte characters. Even in this simple case, it does not work with multibyte strings if the locale encoding is GB18030 and one of the characters to be searched is a digit. */ # undef strcspn /* Assume strcspn is always declared. */ _GL_WARN_ON_USE (strcspn, "strcspn cannot work correctly on character strings " "in multibyte locales - " "use mbscspn if you care about internationalization"); #endif /* Find the first occurrence in S of any character in ACCEPT. */ #if @GNULIB_STRPBRK@ # if ! @HAVE_STRPBRK@ _GL_FUNCDECL_SYS (strpbrk, char *, (char const *__s, char const *__accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); # endif /* On some systems, this function is defined as an overloaded function: extern "C" { const char * strpbrk (const char *, const char *); } extern "C++" { char * strpbrk (char *, const char *); } */ _GL_CXXALIAS_SYS_CAST2 (strpbrk, char *, (char const *__s, char const *__accept), const char *, (char const *__s, char const *__accept)); # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strpbrk, char *, (char *__s, char const *__accept)); _GL_CXXALIASWARN1 (strpbrk, char const *, (char const *__s, char const *__accept)); # else _GL_CXXALIASWARN (strpbrk); # endif # if defined GNULIB_POSIXCHECK /* strpbrk() assumes the second argument is a list of single-byte characters. Even in this simple case, it does not work with multibyte strings if the locale encoding is GB18030 and one of the characters to be searched is a digit. */ # undef strpbrk _GL_WARN_ON_USE (strpbrk, "strpbrk cannot work correctly on character strings " "in multibyte locales - " "use mbspbrk if you care about internationalization"); # endif #elif defined GNULIB_POSIXCHECK # undef strpbrk # if HAVE_RAW_DECL_STRPBRK _GL_WARN_ON_USE (strpbrk, "strpbrk is unportable - " "use gnulib module strpbrk for portability"); # endif #endif #if defined GNULIB_POSIXCHECK /* strspn() assumes the second argument is a list of single-byte characters. Even in this simple case, it cannot work with multibyte strings. */ # undef strspn /* Assume strspn is always declared. */ _GL_WARN_ON_USE (strspn, "strspn cannot work correctly on character strings " "in multibyte locales - " "use mbsspn if you care about internationalization"); #endif #if defined GNULIB_POSIXCHECK /* strrchr() does not work with multibyte strings if the locale encoding is GB18030 and the character to be searched is a digit. */ # undef strrchr /* Assume strrchr is always declared. */ _GL_WARN_ON_USE (strrchr, "strrchr cannot work correctly on character strings " "in some multibyte locales - " "use mbsrchr if you care about internationalization"); #endif /* Search the next delimiter (char listed in DELIM) starting at *STRINGP. If one is found, overwrite it with a NUL, and advance *STRINGP to point to the next char after it. Otherwise, set *STRINGP to NULL. If *STRINGP was already NULL, nothing happens. Return the old value of *STRINGP. This is a variant of strtok() that is multithread-safe and supports empty fields. Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. Caveat: It doesn't work with multibyte strings unless all of the delimiter characters are ASCII characters < 0x30. See also strtok_r(). */ #if @GNULIB_STRSEP@ # if ! @HAVE_STRSEP@ _GL_FUNCDECL_SYS (strsep, char *, (char **restrict __stringp, char const *restrict __delim) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (strsep, char *, (char **restrict __stringp, char const *restrict __delim)); _GL_CXXALIASWARN (strsep); # if defined GNULIB_POSIXCHECK # undef strsep _GL_WARN_ON_USE (strsep, "strsep cannot work correctly on character strings " "in multibyte locales - " "use mbssep if you care about internationalization"); # endif #elif defined GNULIB_POSIXCHECK # undef strsep # if HAVE_RAW_DECL_STRSEP _GL_WARN_ON_USE (strsep, "strsep is unportable - " "use gnulib module strsep for portability"); # endif #endif #if @GNULIB_STRSTR@ # if @REPLACE_STRSTR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strstr rpl_strstr # endif _GL_FUNCDECL_RPL (strstr, char *, (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (strstr, char *, (const char *haystack, const char *needle)); # else /* On some systems, this function is defined as an overloaded function: extern "C++" { const char * strstr (const char *, const char *); } extern "C++" { char * strstr (char *, const char *); } */ _GL_CXXALIAS_SYS_CAST2 (strstr, char *, (const char *haystack, const char *needle), const char *, (const char *haystack, const char *needle)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strstr, char *, (char *haystack, const char *needle)); _GL_CXXALIASWARN1 (strstr, const char *, (const char *haystack, const char *needle)); # else _GL_CXXALIASWARN (strstr); # endif #elif defined GNULIB_POSIXCHECK /* strstr() does not work with multibyte strings if the locale encoding is different from UTF-8: POSIX says that it operates on "strings", and "string" in POSIX is defined as a sequence of bytes, not of characters. */ # undef strstr /* Assume strstr is always declared. */ _GL_WARN_ON_USE (strstr, "strstr is quadratic on many systems, and cannot " "work correctly on character strings in most " "multibyte locales - " "use mbsstr if you care about internationalization, " "or use strstr if you care about speed"); #endif /* Find the first occurrence of NEEDLE in HAYSTACK, using case-insensitive comparison. */ #if @GNULIB_STRCASESTR@ # if @REPLACE_STRCASESTR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strcasestr rpl_strcasestr # endif _GL_FUNCDECL_RPL (strcasestr, char *, (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (strcasestr, char *, (const char *haystack, const char *needle)); # else # if ! @HAVE_STRCASESTR@ _GL_FUNCDECL_SYS (strcasestr, char *, (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); # endif /* On some systems, this function is defined as an overloaded function: extern "C++" { const char * strcasestr (const char *, const char *); } extern "C++" { char * strcasestr (char *, const char *); } */ _GL_CXXALIAS_SYS_CAST2 (strcasestr, char *, (const char *haystack, const char *needle), const char *, (const char *haystack, const char *needle)); # endif # if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 10) && !defined __UCLIBC__) \ && (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) _GL_CXXALIASWARN1 (strcasestr, char *, (char *haystack, const char *needle)); _GL_CXXALIASWARN1 (strcasestr, const char *, (const char *haystack, const char *needle)); # else _GL_CXXALIASWARN (strcasestr); # endif #elif defined GNULIB_POSIXCHECK /* strcasestr() does not work with multibyte strings: It is a glibc extension, and glibc implements it only for unibyte locales. */ # undef strcasestr # if HAVE_RAW_DECL_STRCASESTR _GL_WARN_ON_USE (strcasestr, "strcasestr does work correctly on character " "strings in multibyte locales - " "use mbscasestr if you care about " "internationalization, or use c-strcasestr if you want " "a locale independent function"); # endif #endif /* Parse S into tokens separated by characters in DELIM. If S is NULL, the saved pointer in SAVE_PTR is used as the next starting point. For example: char s[] = "-abc-=-def"; char *sp; x = strtok_r(s, "-", &sp); // x = "abc", sp = "=-def" x = strtok_r(NULL, "-=", &sp); // x = "def", sp = NULL x = strtok_r(NULL, "=", &sp); // x = NULL // s = "abc\0-def\0" This is a variant of strtok() that is multithread-safe. For the POSIX documentation for this function, see: http://www.opengroup.org/susv3xsh/strtok.html Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. Caveat: It doesn't work with multibyte strings unless all of the delimiter characters are ASCII characters < 0x30. See also strsep(). */ #if @GNULIB_STRTOK_R@ # if @REPLACE_STRTOK_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strtok_r # define strtok_r rpl_strtok_r # endif _GL_FUNCDECL_RPL (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr)); # else # if @UNDEFINE_STRTOK_R@ || defined GNULIB_POSIXCHECK # undef strtok_r # endif # if ! @HAVE_DECL_STRTOK_R@ _GL_FUNCDECL_SYS (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr) _GL_ARG_NONNULL ((2, 3))); # endif _GL_CXXALIAS_SYS (strtok_r, char *, (char *restrict s, char const *restrict delim, char **restrict save_ptr)); # endif _GL_CXXALIASWARN (strtok_r); # if defined GNULIB_POSIXCHECK _GL_WARN_ON_USE (strtok_r, "strtok_r cannot work correctly on character " "strings in multibyte locales - " "use mbstok_r if you care about internationalization"); # endif #elif defined GNULIB_POSIXCHECK # undef strtok_r # if HAVE_RAW_DECL_STRTOK_R _GL_WARN_ON_USE (strtok_r, "strtok_r is unportable - " "use gnulib module strtok_r for portability"); # endif #endif /* The following functions are not specified by POSIX. They are gnulib extensions. */ #if @GNULIB_MBSLEN@ /* Return the number of multibyte characters in the character string STRING. This considers multibyte characters, unlike strlen, which counts bytes. */ # ifdef __MirBSD__ /* MirBSD defines mbslen as a macro. Override it. */ # undef mbslen # endif # if @HAVE_MBSLEN@ /* AIX, OSF/1, MirBSD define mbslen already in libc. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbslen rpl_mbslen # endif _GL_FUNCDECL_RPL (mbslen, size_t, (const char *string) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mbslen, size_t, (const char *string)); # else _GL_FUNCDECL_SYS (mbslen, size_t, (const char *string) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (mbslen, size_t, (const char *string)); # endif _GL_CXXALIASWARN (mbslen); #endif #if @GNULIB_MBSNLEN@ /* Return the number of multibyte characters in the character string starting at STRING and ending at STRING + LEN. */ _GL_EXTERN_C size_t mbsnlen (const char *string, size_t len) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1)); #endif #if @GNULIB_MBSCHR@ /* Locate the first single-byte character C in the character string STRING, and return a pointer to it. Return NULL if C is not found in STRING. Unlike strchr(), this function works correctly in multibyte locales with encodings such as GB18030. */ # if defined __hpux # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbschr rpl_mbschr /* avoid collision with HP-UX function */ # endif _GL_FUNCDECL_RPL (mbschr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mbschr, char *, (const char *string, int c)); # else _GL_FUNCDECL_SYS (mbschr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (mbschr, char *, (const char *string, int c)); # endif _GL_CXXALIASWARN (mbschr); #endif #if @GNULIB_MBSRCHR@ /* Locate the last single-byte character C in the character string STRING, and return a pointer to it. Return NULL if C is not found in STRING. Unlike strrchr(), this function works correctly in multibyte locales with encodings such as GB18030. */ # if defined __hpux || defined __INTERIX # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbsrchr rpl_mbsrchr /* avoid collision with system function */ # endif _GL_FUNCDECL_RPL (mbsrchr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mbsrchr, char *, (const char *string, int c)); # else _GL_FUNCDECL_SYS (mbsrchr, char *, (const char *string, int c) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_SYS (mbsrchr, char *, (const char *string, int c)); # endif _GL_CXXALIASWARN (mbsrchr); #endif #if @GNULIB_MBSSTR@ /* Find the first occurrence of the character string NEEDLE in the character string HAYSTACK. Return NULL if NEEDLE is not found in HAYSTACK. Unlike strstr(), this function works correctly in multibyte locales with encodings different from UTF-8. */ _GL_EXTERN_C char * mbsstr (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSCASECMP@ /* Compare the character strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function may, in multibyte locales, return 0 for strings of different lengths! Unlike strcasecmp(), this function works correctly in multibyte locales. */ _GL_EXTERN_C int mbscasecmp (const char *s1, const char *s2) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSNCASECMP@ /* Compare the initial segment of the character string S1 consisting of at most N characters with the initial segment of the character string S2 consisting of at most N characters, ignoring case, returning less than, equal to or greater than zero if the initial segment of S1 is lexicographically less than, equal to or greater than the initial segment of S2. Note: This function may, in multibyte locales, return 0 for initial segments of different lengths! Unlike strncasecmp(), this function works correctly in multibyte locales. But beware that N is not a byte count but a character count! */ _GL_EXTERN_C int mbsncasecmp (const char *s1, const char *s2, size_t n) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSPCASECMP@ /* Compare the initial segment of the character string STRING consisting of at most mbslen (PREFIX) characters with the character string PREFIX, ignoring case. If the two match, return a pointer to the first byte after this prefix in STRING. Otherwise, return NULL. Note: This function may, in multibyte locales, return non-NULL if STRING is of smaller length than PREFIX! Unlike strncasecmp(), this function works correctly in multibyte locales. */ _GL_EXTERN_C char * mbspcasecmp (const char *string, const char *prefix) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSCASESTR@ /* Find the first occurrence of the character string NEEDLE in the character string HAYSTACK, using case-insensitive comparison. Note: This function may, in multibyte locales, return success even if strlen (haystack) < strlen (needle) ! Unlike strcasestr(), this function works correctly in multibyte locales. */ _GL_EXTERN_C char * mbscasestr (const char *haystack, const char *needle) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSCSPN@ /* Find the first occurrence in the character string STRING of any character in the character string ACCEPT. Return the number of bytes from the beginning of the string to this occurrence, or to the end of the string if none exists. Unlike strcspn(), this function works correctly in multibyte locales. */ _GL_EXTERN_C size_t mbscspn (const char *string, const char *accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSPBRK@ /* Find the first occurrence in the character string STRING of any character in the character string ACCEPT. Return the pointer to it, or NULL if none exists. Unlike strpbrk(), this function works correctly in multibyte locales. */ # if defined __hpux # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mbspbrk rpl_mbspbrk /* avoid collision with HP-UX function */ # endif _GL_FUNCDECL_RPL (mbspbrk, char *, (const char *string, const char *accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (mbspbrk, char *, (const char *string, const char *accept)); # else _GL_FUNCDECL_SYS (mbspbrk, char *, (const char *string, const char *accept) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_SYS (mbspbrk, char *, (const char *string, const char *accept)); # endif _GL_CXXALIASWARN (mbspbrk); #endif #if @GNULIB_MBSSPN@ /* Find the first occurrence in the character string STRING of any character not in the character string REJECT. Return the number of bytes from the beginning of the string to this occurrence, or to the end of the string if none exists. Unlike strspn(), this function works correctly in multibyte locales. */ _GL_EXTERN_C size_t mbsspn (const char *string, const char *reject) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSSEP@ /* Search the next delimiter (multibyte character listed in the character string DELIM) starting at the character string *STRINGP. If one is found, overwrite it with a NUL, and advance *STRINGP to point to the next multibyte character after it. Otherwise, set *STRINGP to NULL. If *STRINGP was already NULL, nothing happens. Return the old value of *STRINGP. This is a variant of mbstok_r() that supports empty fields. Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. See also mbstok_r(). */ _GL_EXTERN_C char * mbssep (char **stringp, const char *delim) _GL_ARG_NONNULL ((1, 2)); #endif #if @GNULIB_MBSTOK_R@ /* Parse the character string STRING into tokens separated by characters in the character string DELIM. If STRING is NULL, the saved pointer in SAVE_PTR is used as the next starting point. For example: char s[] = "-abc-=-def"; char *sp; x = mbstok_r(s, "-", &sp); // x = "abc", sp = "=-def" x = mbstok_r(NULL, "-=", &sp); // x = "def", sp = NULL x = mbstok_r(NULL, "=", &sp); // x = NULL // s = "abc\0-def\0" Caveat: It modifies the original string. Caveat: These functions cannot be used on constant strings. Caveat: The identity of the delimiting character is lost. See also mbssep(). */ _GL_EXTERN_C char * mbstok_r (char *string, const char *delim, char **save_ptr) _GL_ARG_NONNULL ((2, 3)); #endif /* Map any int, typically from errno, into an error message. */ #if @GNULIB_STRERROR@ # if @REPLACE_STRERROR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strerror # define strerror rpl_strerror # endif _GL_FUNCDECL_RPL (strerror, char *, (int)); _GL_CXXALIAS_RPL (strerror, char *, (int)); # else _GL_CXXALIAS_SYS (strerror, char *, (int)); # endif _GL_CXXALIASWARN (strerror); #elif defined GNULIB_POSIXCHECK # undef strerror /* Assume strerror is always declared. */ _GL_WARN_ON_USE (strerror, "strerror is unportable - " "use gnulib module strerror to guarantee non-NULL result"); #endif /* Map any int, typically from errno, into an error message. Multithread-safe. Uses the POSIX declaration, not the glibc declaration. */ #if @GNULIB_STRERROR_R@ # if @REPLACE_STRERROR_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strerror_r # define strerror_r rpl_strerror_r # endif _GL_FUNCDECL_RPL (strerror_r, int, (int errnum, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (strerror_r, int, (int errnum, char *buf, size_t buflen)); # else # if !@HAVE_DECL_STRERROR_R@ _GL_FUNCDECL_SYS (strerror_r, int, (int errnum, char *buf, size_t buflen) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (strerror_r, int, (int errnum, char *buf, size_t buflen)); # endif # if @HAVE_DECL_STRERROR_R@ _GL_CXXALIASWARN (strerror_r); # endif #elif defined GNULIB_POSIXCHECK # undef strerror_r # if HAVE_RAW_DECL_STRERROR_R _GL_WARN_ON_USE (strerror_r, "strerror_r is unportable - " "use gnulib module strerror_r-posix for portability"); # endif #endif #if @GNULIB_STRSIGNAL@ # if @REPLACE_STRSIGNAL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strsignal rpl_strsignal # endif _GL_FUNCDECL_RPL (strsignal, char *, (int __sig)); _GL_CXXALIAS_RPL (strsignal, char *, (int __sig)); # else # if ! @HAVE_DECL_STRSIGNAL@ _GL_FUNCDECL_SYS (strsignal, char *, (int __sig)); # endif /* Need to cast, because on Cygwin 1.5.x systems, the return type is 'const char *'. */ _GL_CXXALIAS_SYS_CAST (strsignal, char *, (int __sig)); # endif _GL_CXXALIASWARN (strsignal); #elif defined GNULIB_POSIXCHECK # undef strsignal # if HAVE_RAW_DECL_STRSIGNAL _GL_WARN_ON_USE (strsignal, "strsignal is unportable - " "use gnulib module strsignal for portability"); # endif #endif #if @GNULIB_STRVERSCMP@ # if !@HAVE_STRVERSCMP@ _GL_FUNCDECL_SYS (strverscmp, int, (const char *, const char *) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (strverscmp, int, (const char *, const char *)); _GL_CXXALIASWARN (strverscmp); #elif defined GNULIB_POSIXCHECK # undef strverscmp # if HAVE_RAW_DECL_STRVERSCMP _GL_WARN_ON_USE (strverscmp, "strverscmp is unportable - " "use gnulib module strverscmp for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_STRING_H */ #endif /* _@GUARD_PREFIX@_STRING_H */ #endif gnuastro-0.5/bootstrapped/lib/strerror-override.h0000644000175000017500000000374413217200021017261 00000000000000/* strerror-override.h --- POSIX compatible system error routine Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_STRERROR_OVERRIDE_H # define _GL_STRERROR_OVERRIDE_H # include # include /* Reasonable buffer size that should never trigger ERANGE; if this proves too small, we intentionally abort(), to remind us to fix this value. */ # define STACKBUF_LEN 256 /* If ERRNUM maps to an errno value defined by gnulib, return a string describing the error. Otherwise return NULL. */ # if REPLACE_STRERROR_0 \ || GNULIB_defined_ESOCK \ || GNULIB_defined_ESTREAMS \ || GNULIB_defined_EWINSOCK \ || GNULIB_defined_ENOMSG \ || GNULIB_defined_EIDRM \ || GNULIB_defined_ENOLINK \ || GNULIB_defined_EPROTO \ || GNULIB_defined_EMULTIHOP \ || GNULIB_defined_EBADMSG \ || GNULIB_defined_EOVERFLOW \ || GNULIB_defined_ENOTSUP \ || GNULIB_defined_ENETRESET \ || GNULIB_defined_ECONNABORTED \ || GNULIB_defined_ESTALE \ || GNULIB_defined_EDQUOT \ || GNULIB_defined_ECANCELED \ || GNULIB_defined_EOWNERDEAD \ || GNULIB_defined_ENOTRECOVERABLE \ || GNULIB_defined_EILSEQ extern const char *strerror_override (int errnum) _GL_ATTRIBUTE_CONST; # else # define strerror_override(ignored) NULL # endif #endif /* _GL_STRERROR_OVERRIDE_H */ gnuastro-0.5/bootstrapped/lib/streq.h0000644000175000017500000000763713217200021014725 00000000000000/* Optimized string comparison. Copyright (C) 2001-2002, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible . */ #ifndef _GL_STREQ_H #define _GL_STREQ_H #include /* STREQ_OPT allows to optimize string comparison with a small literal string. STREQ_OPT (s, "EUC-KR", 'E', 'U', 'C', '-', 'K', 'R', 0, 0, 0) is semantically equivalent to strcmp (s, "EUC-KR") == 0 just faster. */ /* Help GCC to generate good code for string comparisons with immediate strings. */ #if defined (__GNUC__) && defined (__OPTIMIZE__) static inline int streq9 (const char *s1, const char *s2) { return strcmp (s1 + 9, s2 + 9) == 0; } static inline int streq8 (const char *s1, const char *s2, char s28) { if (s1[8] == s28) { if (s28 == 0) return 1; else return streq9 (s1, s2); } else return 0; } static inline int streq7 (const char *s1, const char *s2, char s27, char s28) { if (s1[7] == s27) { if (s27 == 0) return 1; else return streq8 (s1, s2, s28); } else return 0; } static inline int streq6 (const char *s1, const char *s2, char s26, char s27, char s28) { if (s1[6] == s26) { if (s26 == 0) return 1; else return streq7 (s1, s2, s27, s28); } else return 0; } static inline int streq5 (const char *s1, const char *s2, char s25, char s26, char s27, char s28) { if (s1[5] == s25) { if (s25 == 0) return 1; else return streq6 (s1, s2, s26, s27, s28); } else return 0; } static inline int streq4 (const char *s1, const char *s2, char s24, char s25, char s26, char s27, char s28) { if (s1[4] == s24) { if (s24 == 0) return 1; else return streq5 (s1, s2, s25, s26, s27, s28); } else return 0; } static inline int streq3 (const char *s1, const char *s2, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[3] == s23) { if (s23 == 0) return 1; else return streq4 (s1, s2, s24, s25, s26, s27, s28); } else return 0; } static inline int streq2 (const char *s1, const char *s2, char s22, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[2] == s22) { if (s22 == 0) return 1; else return streq3 (s1, s2, s23, s24, s25, s26, s27, s28); } else return 0; } static inline int streq1 (const char *s1, const char *s2, char s21, char s22, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[1] == s21) { if (s21 == 0) return 1; else return streq2 (s1, s2, s22, s23, s24, s25, s26, s27, s28); } else return 0; } static inline int streq0 (const char *s1, const char *s2, char s20, char s21, char s22, char s23, char s24, char s25, char s26, char s27, char s28) { if (s1[0] == s20) { if (s20 == 0) return 1; else return streq1 (s1, s2, s21, s22, s23, s24, s25, s26, s27, s28); } else return 0; } #define STREQ_OPT(s1,s2,s20,s21,s22,s23,s24,s25,s26,s27,s28) \ streq0 (s1, s2, s20, s21, s22, s23, s24, s25, s26, s27, s28) #else #define STREQ_OPT(s1,s2,s20,s21,s22,s23,s24,s25,s26,s27,s28) \ (strcmp (s1, s2) == 0) #endif #endif /* _GL_STREQ_H */ gnuastro-0.5/bootstrapped/lib/strchrnul.valgrind0000644000175000017500000000040313217200021017152 00000000000000# Suppress a valgrind message about use of uninitialized memory in strchrnul(). # This use is OK because it provides only a speedup. { strchrnul-value4 Memcheck:Value4 fun:strchrnul } { strchrnul-value8 Memcheck:Value8 fun:strchrnul } gnuastro-0.5/bootstrapped/lib/stdlib.in.h0000644000175000017500000010501513217200021015442 00000000000000/* A GNU-like . Copyright (C) 1995, 2001-2004, 2006-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_system_stdlib_h || defined __need_malloc_and_calloc /* Special invocation conventions inside some gnulib header files, and inside some glibc header files, respectively. */ #@INCLUDE_NEXT@ @NEXT_STDLIB_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_STDLIB_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_STDLIB_H@ #ifndef _@GUARD_PREFIX@_STDLIB_H #define _@GUARD_PREFIX@_STDLIB_H /* NetBSD 5.0 mis-defines NULL. */ #include /* MirBSD 10 defines WEXITSTATUS in , not in . */ #if @GNULIB_SYSTEM_POSIX@ && !defined WEXITSTATUS # include #endif /* Solaris declares getloadavg() in . */ #if (@GNULIB_GETLOADAVG@ || defined GNULIB_POSIXCHECK) && @HAVE_SYS_LOADAVG_H@ # include #endif /* Native Windows platforms declare mktemp() in . */ #if 0 && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) # include #endif #if @GNULIB_RANDOM_R@ /* OSF/1 5.1 declares 'struct random_data' in , which is included from if _REENTRANT is defined. Include it whenever we need 'struct random_data'. */ # if @HAVE_RANDOM_H@ # include # endif # if !@HAVE_STRUCT_RANDOM_DATA@ || @REPLACE_RANDOM_R@ || !@HAVE_RANDOM_R@ # include # endif # if !@HAVE_STRUCT_RANDOM_DATA@ /* Define 'struct random_data'. But allow multiple gnulib generated replacements to coexist. */ # if !GNULIB_defined_struct_random_data struct random_data { int32_t *fptr; /* Front pointer. */ int32_t *rptr; /* Rear pointer. */ int32_t *state; /* Array of state values. */ int rand_type; /* Type of random number generator. */ int rand_deg; /* Degree of random number generator. */ int rand_sep; /* Distance between front and rear. */ int32_t *end_ptr; /* Pointer behind state table. */ }; # define GNULIB_defined_struct_random_data 1 # endif # endif #endif #if (@GNULIB_MKSTEMP@ || @GNULIB_MKSTEMPS@ || @GNULIB_GETSUBOPT@ || defined GNULIB_POSIXCHECK) && ! defined __GLIBC__ && !((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) /* On Mac OS X 10.3, only declares mkstemp. */ /* On Mac OS X 10.5, only declares mkstemps. */ /* On Cygwin 1.7.1, only declares getsubopt. */ /* But avoid namespace pollution on glibc systems and native Windows. */ # include #endif /* The __attribute__ feature is available in gcc versions 2.5 and later. The attribute __pure__ was added in gcc 2.96. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 96) # define _GL_ATTRIBUTE_PURE __attribute__ ((__pure__)) #else # define _GL_ATTRIBUTE_PURE /* empty */ #endif /* The definition of _Noreturn is copied here. */ /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Some systems do not define EXIT_*, despite otherwise supporting C89. */ #ifndef EXIT_SUCCESS # define EXIT_SUCCESS 0 #endif /* Tandem/NSK and other platforms that define EXIT_FAILURE as -1 interfere with proper operation of xargs. */ #ifndef EXIT_FAILURE # define EXIT_FAILURE 1 #elif EXIT_FAILURE != 1 # undef EXIT_FAILURE # define EXIT_FAILURE 1 #endif #if @GNULIB__EXIT@ /* Terminate the current process with the given return code, without running the 'atexit' handlers. */ # if !@HAVE__EXIT@ _GL_FUNCDECL_SYS (_Exit, _Noreturn void, (int status)); # endif _GL_CXXALIAS_SYS (_Exit, void, (int status)); _GL_CXXALIASWARN (_Exit); #elif defined GNULIB_POSIXCHECK # undef _Exit # if HAVE_RAW_DECL__EXIT _GL_WARN_ON_USE (_Exit, "_Exit is unportable - " "use gnulib module _Exit for portability"); # endif #endif #if @GNULIB_ATOLL@ /* Parse a signed decimal integer. Returns the value of the integer. Errors are not detected. */ # if !@HAVE_ATOLL@ _GL_FUNCDECL_SYS (atoll, long long, (const char *string) _GL_ATTRIBUTE_PURE _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (atoll, long long, (const char *string)); _GL_CXXALIASWARN (atoll); #elif defined GNULIB_POSIXCHECK # undef atoll # if HAVE_RAW_DECL_ATOLL _GL_WARN_ON_USE (atoll, "atoll is unportable - " "use gnulib module atoll for portability"); # endif #endif #if @GNULIB_CALLOC_POSIX@ # if @REPLACE_CALLOC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef calloc # define calloc rpl_calloc # endif _GL_FUNCDECL_RPL (calloc, void *, (size_t nmemb, size_t size)); _GL_CXXALIAS_RPL (calloc, void *, (size_t nmemb, size_t size)); # else _GL_CXXALIAS_SYS (calloc, void *, (size_t nmemb, size_t size)); # endif _GL_CXXALIASWARN (calloc); #elif defined GNULIB_POSIXCHECK # undef calloc /* Assume calloc is always declared. */ _GL_WARN_ON_USE (calloc, "calloc is not POSIX compliant everywhere - " "use gnulib module calloc-posix for portability"); #endif #if @GNULIB_CANONICALIZE_FILE_NAME@ # if @REPLACE_CANONICALIZE_FILE_NAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define canonicalize_file_name rpl_canonicalize_file_name # endif _GL_FUNCDECL_RPL (canonicalize_file_name, char *, (const char *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (canonicalize_file_name, char *, (const char *name)); # else # if !@HAVE_CANONICALIZE_FILE_NAME@ _GL_FUNCDECL_SYS (canonicalize_file_name, char *, (const char *name) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (canonicalize_file_name, char *, (const char *name)); # endif _GL_CXXALIASWARN (canonicalize_file_name); #elif defined GNULIB_POSIXCHECK # undef canonicalize_file_name # if HAVE_RAW_DECL_CANONICALIZE_FILE_NAME _GL_WARN_ON_USE (canonicalize_file_name, "canonicalize_file_name is unportable - " "use gnulib module canonicalize-lgpl for portability"); # endif #endif #if @GNULIB_GETLOADAVG@ /* Store max(NELEM,3) load average numbers in LOADAVG[]. The three numbers are the load average of the last 1 minute, the last 5 minutes, and the last 15 minutes, respectively. LOADAVG is an array of NELEM numbers. */ # if !@HAVE_DECL_GETLOADAVG@ _GL_FUNCDECL_SYS (getloadavg, int, (double loadavg[], int nelem) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (getloadavg, int, (double loadavg[], int nelem)); _GL_CXXALIASWARN (getloadavg); #elif defined GNULIB_POSIXCHECK # undef getloadavg # if HAVE_RAW_DECL_GETLOADAVG _GL_WARN_ON_USE (getloadavg, "getloadavg is not portable - " "use gnulib module getloadavg for portability"); # endif #endif #if @GNULIB_GETSUBOPT@ /* Assuming *OPTIONP is a comma separated list of elements of the form "token" or "token=value", getsubopt parses the first of these elements. If the first element refers to a "token" that is member of the given NULL-terminated array of tokens: - It replaces the comma with a NUL byte, updates *OPTIONP to point past the first option and the comma, sets *VALUEP to the value of the element (or NULL if it doesn't contain an "=" sign), - It returns the index of the "token" in the given array of tokens. Otherwise it returns -1, and *OPTIONP and *VALUEP are undefined. For more details see the POSIX:2001 specification. http://www.opengroup.org/susv3xsh/getsubopt.html */ # if !@HAVE_GETSUBOPT@ _GL_FUNCDECL_SYS (getsubopt, int, (char **optionp, char *const *tokens, char **valuep) _GL_ARG_NONNULL ((1, 2, 3))); # endif _GL_CXXALIAS_SYS (getsubopt, int, (char **optionp, char *const *tokens, char **valuep)); _GL_CXXALIASWARN (getsubopt); #elif defined GNULIB_POSIXCHECK # undef getsubopt # if HAVE_RAW_DECL_GETSUBOPT _GL_WARN_ON_USE (getsubopt, "getsubopt is unportable - " "use gnulib module getsubopt for portability"); # endif #endif #if @GNULIB_GRANTPT@ /* Change the ownership and access permission of the slave side of the pseudo-terminal whose master side is specified by FD. */ # if !@HAVE_GRANTPT@ _GL_FUNCDECL_SYS (grantpt, int, (int fd)); # endif _GL_CXXALIAS_SYS (grantpt, int, (int fd)); _GL_CXXALIASWARN (grantpt); #elif defined GNULIB_POSIXCHECK # undef grantpt # if HAVE_RAW_DECL_GRANTPT _GL_WARN_ON_USE (grantpt, "grantpt is not portable - " "use gnulib module grantpt for portability"); # endif #endif /* If _GL_USE_STDLIB_ALLOC is nonzero, the including module does not rely on GNU or POSIX semantics for malloc and realloc (for example, by never specifying a zero size), so it does not need malloc or realloc to be redefined. */ #if @GNULIB_MALLOC_POSIX@ # if @REPLACE_MALLOC@ # if !((defined __cplusplus && defined GNULIB_NAMESPACE) \ || _GL_USE_STDLIB_ALLOC) # undef malloc # define malloc rpl_malloc # endif _GL_FUNCDECL_RPL (malloc, void *, (size_t size)); _GL_CXXALIAS_RPL (malloc, void *, (size_t size)); # else _GL_CXXALIAS_SYS (malloc, void *, (size_t size)); # endif _GL_CXXALIASWARN (malloc); #elif defined GNULIB_POSIXCHECK && !_GL_USE_STDLIB_ALLOC # undef malloc /* Assume malloc is always declared. */ _GL_WARN_ON_USE (malloc, "malloc is not POSIX compliant everywhere - " "use gnulib module malloc-posix for portability"); #endif /* Convert a multibyte character to a wide character. */ #if @GNULIB_MBTOWC@ # if @REPLACE_MBTOWC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef mbtowc # define mbtowc rpl_mbtowc # endif _GL_FUNCDECL_RPL (mbtowc, int, (wchar_t *pwc, const char *s, size_t n)); _GL_CXXALIAS_RPL (mbtowc, int, (wchar_t *pwc, const char *s, size_t n)); # else _GL_CXXALIAS_SYS (mbtowc, int, (wchar_t *pwc, const char *s, size_t n)); # endif _GL_CXXALIASWARN (mbtowc); #endif #if @GNULIB_MKDTEMP@ /* Create a unique temporary directory from TEMPLATE. The last six characters of TEMPLATE must be "XXXXXX"; they are replaced with a string that makes the directory name unique. Returns TEMPLATE, or a null pointer if it cannot get a unique name. The directory is created mode 700. */ # if !@HAVE_MKDTEMP@ _GL_FUNCDECL_SYS (mkdtemp, char *, (char * /*template*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkdtemp, char *, (char * /*template*/)); _GL_CXXALIASWARN (mkdtemp); #elif defined GNULIB_POSIXCHECK # undef mkdtemp # if HAVE_RAW_DECL_MKDTEMP _GL_WARN_ON_USE (mkdtemp, "mkdtemp is unportable - " "use gnulib module mkdtemp for portability"); # endif #endif #if @GNULIB_MKOSTEMP@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE must be "XXXXXX"; they are replaced with a string that makes the file name unique. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). The file is then created, with the specified flags, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if !@HAVE_MKOSTEMP@ _GL_FUNCDECL_SYS (mkostemp, int, (char * /*template*/, int /*flags*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkostemp, int, (char * /*template*/, int /*flags*/)); _GL_CXXALIASWARN (mkostemp); #elif defined GNULIB_POSIXCHECK # undef mkostemp # if HAVE_RAW_DECL_MKOSTEMP _GL_WARN_ON_USE (mkostemp, "mkostemp is unportable - " "use gnulib module mkostemp for portability"); # endif #endif #if @GNULIB_MKOSTEMPS@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE before a suffix of length SUFFIXLEN must be "XXXXXX"; they are replaced with a string that makes the file name unique. The flags are a bitmask, possibly including O_CLOEXEC (defined in ) and O_TEXT, O_BINARY (defined in "binary-io.h"). The file is then created, with the specified flags, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if !@HAVE_MKOSTEMPS@ _GL_FUNCDECL_SYS (mkostemps, int, (char * /*template*/, int /*suffixlen*/, int /*flags*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkostemps, int, (char * /*template*/, int /*suffixlen*/, int /*flags*/)); _GL_CXXALIASWARN (mkostemps); #elif defined GNULIB_POSIXCHECK # undef mkostemps # if HAVE_RAW_DECL_MKOSTEMPS _GL_WARN_ON_USE (mkostemps, "mkostemps is unportable - " "use gnulib module mkostemps for portability"); # endif #endif #if @GNULIB_MKSTEMP@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE must be "XXXXXX"; they are replaced with a string that makes the file name unique. The file is then created, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if @REPLACE_MKSTEMP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define mkstemp rpl_mkstemp # endif _GL_FUNCDECL_RPL (mkstemp, int, (char * /*template*/) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (mkstemp, int, (char * /*template*/)); # else # if ! @HAVE_MKSTEMP@ _GL_FUNCDECL_SYS (mkstemp, int, (char * /*template*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkstemp, int, (char * /*template*/)); # endif _GL_CXXALIASWARN (mkstemp); #elif defined GNULIB_POSIXCHECK # undef mkstemp # if HAVE_RAW_DECL_MKSTEMP _GL_WARN_ON_USE (mkstemp, "mkstemp is unportable - " "use gnulib module mkstemp for portability"); # endif #endif #if @GNULIB_MKSTEMPS@ /* Create a unique temporary file from TEMPLATE. The last six characters of TEMPLATE prior to a suffix of length SUFFIXLEN must be "XXXXXX"; they are replaced with a string that makes the file name unique. The file is then created, ensuring it didn't exist before. The file is created read-write (mask at least 0600 & ~umask), but it may be world-readable and world-writable (mask 0666 & ~umask), depending on the implementation. Returns the open file descriptor if successful, otherwise -1 and errno set. */ # if !@HAVE_MKSTEMPS@ _GL_FUNCDECL_SYS (mkstemps, int, (char * /*template*/, int /*suffixlen*/) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (mkstemps, int, (char * /*template*/, int /*suffixlen*/)); _GL_CXXALIASWARN (mkstemps); #elif defined GNULIB_POSIXCHECK # undef mkstemps # if HAVE_RAW_DECL_MKSTEMPS _GL_WARN_ON_USE (mkstemps, "mkstemps is unportable - " "use gnulib module mkstemps for portability"); # endif #endif #if @GNULIB_POSIX_OPENPT@ /* Return an FD open to the master side of a pseudo-terminal. Flags should include O_RDWR, and may also include O_NOCTTY. */ # if !@HAVE_POSIX_OPENPT@ _GL_FUNCDECL_SYS (posix_openpt, int, (int flags)); # endif _GL_CXXALIAS_SYS (posix_openpt, int, (int flags)); _GL_CXXALIASWARN (posix_openpt); #elif defined GNULIB_POSIXCHECK # undef posix_openpt # if HAVE_RAW_DECL_POSIX_OPENPT _GL_WARN_ON_USE (posix_openpt, "posix_openpt is not portable - " "use gnulib module posix_openpt for portability"); # endif #endif #if @GNULIB_PTSNAME@ /* Return the pathname of the pseudo-terminal slave associated with the master FD is open on, or NULL on errors. */ # if @REPLACE_PTSNAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ptsname # define ptsname rpl_ptsname # endif _GL_FUNCDECL_RPL (ptsname, char *, (int fd)); _GL_CXXALIAS_RPL (ptsname, char *, (int fd)); # else # if !@HAVE_PTSNAME@ _GL_FUNCDECL_SYS (ptsname, char *, (int fd)); # endif _GL_CXXALIAS_SYS (ptsname, char *, (int fd)); # endif _GL_CXXALIASWARN (ptsname); #elif defined GNULIB_POSIXCHECK # undef ptsname # if HAVE_RAW_DECL_PTSNAME _GL_WARN_ON_USE (ptsname, "ptsname is not portable - " "use gnulib module ptsname for portability"); # endif #endif #if @GNULIB_PTSNAME_R@ /* Set the pathname of the pseudo-terminal slave associated with the master FD is open on and return 0, or set errno and return non-zero on errors. */ # if @REPLACE_PTSNAME_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ptsname_r # define ptsname_r rpl_ptsname_r # endif _GL_FUNCDECL_RPL (ptsname_r, int, (int fd, char *buf, size_t len)); _GL_CXXALIAS_RPL (ptsname_r, int, (int fd, char *buf, size_t len)); # else # if !@HAVE_PTSNAME_R@ _GL_FUNCDECL_SYS (ptsname_r, int, (int fd, char *buf, size_t len)); # endif _GL_CXXALIAS_SYS (ptsname_r, int, (int fd, char *buf, size_t len)); # endif _GL_CXXALIASWARN (ptsname_r); #elif defined GNULIB_POSIXCHECK # undef ptsname_r # if HAVE_RAW_DECL_PTSNAME_R _GL_WARN_ON_USE (ptsname_r, "ptsname_r is not portable - " "use gnulib module ptsname_r for portability"); # endif #endif #if @GNULIB_PUTENV@ # if @REPLACE_PUTENV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef putenv # define putenv rpl_putenv # endif _GL_FUNCDECL_RPL (putenv, int, (char *string) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (putenv, int, (char *string)); # else _GL_CXXALIAS_SYS (putenv, int, (char *string)); # endif _GL_CXXALIASWARN (putenv); #endif #if @GNULIB_QSORT_R@ /* Sort an array of NMEMB elements, starting at address BASE, each element occupying SIZE bytes, in ascending order according to the comparison function COMPARE. */ # if @REPLACE_QSORT_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef qsort_r # define qsort_r rpl_qsort_r # endif _GL_FUNCDECL_RPL (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg) _GL_ARG_NONNULL ((1, 4))); _GL_CXXALIAS_RPL (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg)); # else # if !@HAVE_QSORT_R@ _GL_FUNCDECL_SYS (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg) _GL_ARG_NONNULL ((1, 4))); # endif _GL_CXXALIAS_SYS (qsort_r, void, (void *base, size_t nmemb, size_t size, int (*compare) (void const *, void const *, void *), void *arg)); # endif _GL_CXXALIASWARN (qsort_r); #elif defined GNULIB_POSIXCHECK # undef qsort_r # if HAVE_RAW_DECL_QSORT_R _GL_WARN_ON_USE (qsort_r, "qsort_r is not portable - " "use gnulib module qsort_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if !@HAVE_RANDOM_R@ # ifndef RAND_MAX # define RAND_MAX 2147483647 # endif # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ _GL_FUNCDECL_SYS (random, long, (void)); # endif _GL_CXXALIAS_SYS (random, long, (void)); _GL_CXXALIASWARN (random); #elif defined GNULIB_POSIXCHECK # undef random # if HAVE_RAW_DECL_RANDOM _GL_WARN_ON_USE (random, "random is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ _GL_FUNCDECL_SYS (srandom, void, (unsigned int seed)); # endif _GL_CXXALIAS_SYS (srandom, void, (unsigned int seed)); _GL_CXXALIASWARN (srandom); #elif defined GNULIB_POSIXCHECK # undef srandom # if HAVE_RAW_DECL_SRANDOM _GL_WARN_ON_USE (srandom, "srandom is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ || !@HAVE_DECL_INITSTATE@ _GL_FUNCDECL_SYS (initstate, char *, (unsigned int seed, char *buf, size_t buf_size) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (initstate, char *, (unsigned int seed, char *buf, size_t buf_size)); _GL_CXXALIASWARN (initstate); #elif defined GNULIB_POSIXCHECK # undef initstate # if HAVE_RAW_DECL_INITSTATE_R _GL_WARN_ON_USE (initstate, "initstate is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM@ # if !@HAVE_RANDOM@ || !@HAVE_DECL_SETSTATE@ _GL_FUNCDECL_SYS (setstate, char *, (char *arg_state) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (setstate, char *, (char *arg_state)); _GL_CXXALIASWARN (setstate); #elif defined GNULIB_POSIXCHECK # undef setstate # if HAVE_RAW_DECL_SETSTATE_R _GL_WARN_ON_USE (setstate, "setstate is unportable - " "use gnulib module random for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef random_r # define random_r rpl_random_r # endif _GL_FUNCDECL_RPL (random_r, int, (struct random_data *buf, int32_t *result) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (random_r, int, (struct random_data *buf, int32_t *result)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (random_r, int, (struct random_data *buf, int32_t *result) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (random_r, int, (struct random_data *buf, int32_t *result)); # endif _GL_CXXALIASWARN (random_r); #elif defined GNULIB_POSIXCHECK # undef random_r # if HAVE_RAW_DECL_RANDOM_R _GL_WARN_ON_USE (random_r, "random_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef srandom_r # define srandom_r rpl_srandom_r # endif _GL_FUNCDECL_RPL (srandom_r, int, (unsigned int seed, struct random_data *rand_state) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (srandom_r, int, (unsigned int seed, struct random_data *rand_state)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (srandom_r, int, (unsigned int seed, struct random_data *rand_state) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (srandom_r, int, (unsigned int seed, struct random_data *rand_state)); # endif _GL_CXXALIASWARN (srandom_r); #elif defined GNULIB_POSIXCHECK # undef srandom_r # if HAVE_RAW_DECL_SRANDOM_R _GL_WARN_ON_USE (srandom_r, "srandom_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef initstate_r # define initstate_r rpl_initstate_r # endif _GL_FUNCDECL_RPL (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state) _GL_ARG_NONNULL ((2, 4))); _GL_CXXALIAS_RPL (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state) _GL_ARG_NONNULL ((2, 4))); # endif _GL_CXXALIAS_SYS (initstate_r, int, (unsigned int seed, char *buf, size_t buf_size, struct random_data *rand_state)); # endif _GL_CXXALIASWARN (initstate_r); #elif defined GNULIB_POSIXCHECK # undef initstate_r # if HAVE_RAW_DECL_INITSTATE_R _GL_WARN_ON_USE (initstate_r, "initstate_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_RANDOM_R@ # if @REPLACE_RANDOM_R@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setstate_r # define setstate_r rpl_setstate_r # endif _GL_FUNCDECL_RPL (setstate_r, int, (char *arg_state, struct random_data *rand_state) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (setstate_r, int, (char *arg_state, struct random_data *rand_state)); # else # if !@HAVE_RANDOM_R@ _GL_FUNCDECL_SYS (setstate_r, int, (char *arg_state, struct random_data *rand_state) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (setstate_r, int, (char *arg_state, struct random_data *rand_state)); # endif _GL_CXXALIASWARN (setstate_r); #elif defined GNULIB_POSIXCHECK # undef setstate_r # if HAVE_RAW_DECL_SETSTATE_R _GL_WARN_ON_USE (setstate_r, "setstate_r is unportable - " "use gnulib module random_r for portability"); # endif #endif #if @GNULIB_REALLOC_POSIX@ # if @REPLACE_REALLOC@ # if !((defined __cplusplus && defined GNULIB_NAMESPACE) \ || _GL_USE_STDLIB_ALLOC) # undef realloc # define realloc rpl_realloc # endif _GL_FUNCDECL_RPL (realloc, void *, (void *ptr, size_t size)); _GL_CXXALIAS_RPL (realloc, void *, (void *ptr, size_t size)); # else _GL_CXXALIAS_SYS (realloc, void *, (void *ptr, size_t size)); # endif _GL_CXXALIASWARN (realloc); #elif defined GNULIB_POSIXCHECK && !_GL_USE_STDLIB_ALLOC # undef realloc /* Assume realloc is always declared. */ _GL_WARN_ON_USE (realloc, "realloc is not POSIX compliant everywhere - " "use gnulib module realloc-posix for portability"); #endif #if @GNULIB_REALLOCARRAY@ # if ! @HAVE_REALLOCARRAY@ _GL_FUNCDECL_SYS (reallocarray, void *, (void *ptr, size_t nmemb, size_t size)); # endif _GL_CXXALIAS_SYS (reallocarray, void *, (void *ptr, size_t nmemb, size_t size)); _GL_CXXALIASWARN (reallocarray); #elif defined GNULIB_POSIXCHECK # undef reallocarray # if HAVE_RAW_DECL_REALLOCARRAY _GL_WARN_ON_USE (reallocarray, "reallocarray is not portable - " "use gnulib module reallocarray for portability"); # endif #endif #if @GNULIB_REALPATH@ # if @REPLACE_REALPATH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define realpath rpl_realpath # endif _GL_FUNCDECL_RPL (realpath, char *, (const char *name, char *resolved) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (realpath, char *, (const char *name, char *resolved)); # else # if !@HAVE_REALPATH@ _GL_FUNCDECL_SYS (realpath, char *, (const char *name, char *resolved) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (realpath, char *, (const char *name, char *resolved)); # endif _GL_CXXALIASWARN (realpath); #elif defined GNULIB_POSIXCHECK # undef realpath # if HAVE_RAW_DECL_REALPATH _GL_WARN_ON_USE (realpath, "realpath is unportable - use gnulib module " "canonicalize or canonicalize-lgpl for portability"); # endif #endif #if @GNULIB_RPMATCH@ /* Test a user response to a question. Return 1 if it is affirmative, 0 if it is negative, or -1 if not clear. */ # if !@HAVE_RPMATCH@ _GL_FUNCDECL_SYS (rpmatch, int, (const char *response) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (rpmatch, int, (const char *response)); _GL_CXXALIASWARN (rpmatch); #elif defined GNULIB_POSIXCHECK # undef rpmatch # if HAVE_RAW_DECL_RPMATCH _GL_WARN_ON_USE (rpmatch, "rpmatch is unportable - " "use gnulib module rpmatch for portability"); # endif #endif #if @GNULIB_SECURE_GETENV@ /* Look up NAME in the environment, returning 0 in insecure situations. */ # if !@HAVE_SECURE_GETENV@ _GL_FUNCDECL_SYS (secure_getenv, char *, (char const *name) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (secure_getenv, char *, (char const *name)); _GL_CXXALIASWARN (secure_getenv); #elif defined GNULIB_POSIXCHECK # undef secure_getenv # if HAVE_RAW_DECL_SECURE_GETENV _GL_WARN_ON_USE (secure_getenv, "secure_getenv is unportable - " "use gnulib module secure_getenv for portability"); # endif #endif #if @GNULIB_SETENV@ /* Set NAME to VALUE in the environment. If REPLACE is nonzero, overwrite an existing value. */ # if @REPLACE_SETENV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setenv # define setenv rpl_setenv # endif _GL_FUNCDECL_RPL (setenv, int, (const char *name, const char *value, int replace) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (setenv, int, (const char *name, const char *value, int replace)); # else # if !@HAVE_DECL_SETENV@ _GL_FUNCDECL_SYS (setenv, int, (const char *name, const char *value, int replace) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (setenv, int, (const char *name, const char *value, int replace)); # endif # if !(@REPLACE_SETENV@ && !@HAVE_DECL_SETENV@) _GL_CXXALIASWARN (setenv); # endif #elif defined GNULIB_POSIXCHECK # undef setenv # if HAVE_RAW_DECL_SETENV _GL_WARN_ON_USE (setenv, "setenv is unportable - " "use gnulib module setenv for portability"); # endif #endif #if @GNULIB_STRTOD@ /* Parse a double from STRING, updating ENDP if appropriate. */ # if @REPLACE_STRTOD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define strtod rpl_strtod # endif _GL_FUNCDECL_RPL (strtod, double, (const char *str, char **endp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strtod, double, (const char *str, char **endp)); # else # if !@HAVE_STRTOD@ _GL_FUNCDECL_SYS (strtod, double, (const char *str, char **endp) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtod, double, (const char *str, char **endp)); # endif _GL_CXXALIASWARN (strtod); #elif defined GNULIB_POSIXCHECK # undef strtod # if HAVE_RAW_DECL_STRTOD _GL_WARN_ON_USE (strtod, "strtod is unportable - " "use gnulib module strtod for portability"); # endif #endif #if @GNULIB_STRTOLL@ /* Parse a signed integer whose textual representation starts at STRING. The integer is expected to be in base BASE (2 <= BASE <= 36); if BASE == 0, it may be decimal or octal (with prefix "0") or hexadecimal (with prefix "0x"). If ENDPTR is not NULL, the address of the first byte after the integer is stored in *ENDPTR. Upon overflow, the return value is LLONG_MAX or LLONG_MIN, and errno is set to ERANGE. */ # if !@HAVE_STRTOLL@ _GL_FUNCDECL_SYS (strtoll, long long, (const char *string, char **endptr, int base) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoll, long long, (const char *string, char **endptr, int base)); _GL_CXXALIASWARN (strtoll); #elif defined GNULIB_POSIXCHECK # undef strtoll # if HAVE_RAW_DECL_STRTOLL _GL_WARN_ON_USE (strtoll, "strtoll is unportable - " "use gnulib module strtoll for portability"); # endif #endif #if @GNULIB_STRTOULL@ /* Parse an unsigned integer whose textual representation starts at STRING. The integer is expected to be in base BASE (2 <= BASE <= 36); if BASE == 0, it may be decimal or octal (with prefix "0") or hexadecimal (with prefix "0x"). If ENDPTR is not NULL, the address of the first byte after the integer is stored in *ENDPTR. Upon overflow, the return value is ULLONG_MAX, and errno is set to ERANGE. */ # if !@HAVE_STRTOULL@ _GL_FUNCDECL_SYS (strtoull, unsigned long long, (const char *string, char **endptr, int base) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoull, unsigned long long, (const char *string, char **endptr, int base)); _GL_CXXALIASWARN (strtoull); #elif defined GNULIB_POSIXCHECK # undef strtoull # if HAVE_RAW_DECL_STRTOULL _GL_WARN_ON_USE (strtoull, "strtoull is unportable - " "use gnulib module strtoull for portability"); # endif #endif #if @GNULIB_UNLOCKPT@ /* Unlock the slave side of the pseudo-terminal whose master side is specified by FD, so that it can be opened. */ # if !@HAVE_UNLOCKPT@ _GL_FUNCDECL_SYS (unlockpt, int, (int fd)); # endif _GL_CXXALIAS_SYS (unlockpt, int, (int fd)); _GL_CXXALIASWARN (unlockpt); #elif defined GNULIB_POSIXCHECK # undef unlockpt # if HAVE_RAW_DECL_UNLOCKPT _GL_WARN_ON_USE (unlockpt, "unlockpt is not portable - " "use gnulib module unlockpt for portability"); # endif #endif #if @GNULIB_UNSETENV@ /* Remove the variable NAME from the environment. */ # if @REPLACE_UNSETENV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef unsetenv # define unsetenv rpl_unsetenv # endif _GL_FUNCDECL_RPL (unsetenv, int, (const char *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (unsetenv, int, (const char *name)); # else # if !@HAVE_DECL_UNSETENV@ _GL_FUNCDECL_SYS (unsetenv, int, (const char *name) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (unsetenv, int, (const char *name)); # endif # if !(@REPLACE_UNSETENV@ && !@HAVE_DECL_UNSETENV@) _GL_CXXALIASWARN (unsetenv); # endif #elif defined GNULIB_POSIXCHECK # undef unsetenv # if HAVE_RAW_DECL_UNSETENV _GL_WARN_ON_USE (unsetenv, "unsetenv is unportable - " "use gnulib module unsetenv for portability"); # endif #endif /* Convert a wide character to a multibyte character. */ #if @GNULIB_WCTOMB@ # if @REPLACE_WCTOMB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef wctomb # define wctomb rpl_wctomb # endif _GL_FUNCDECL_RPL (wctomb, int, (char *s, wchar_t wc)); _GL_CXXALIAS_RPL (wctomb, int, (char *s, wchar_t wc)); # else _GL_CXXALIAS_SYS (wctomb, int, (char *s, wchar_t wc)); # endif _GL_CXXALIASWARN (wctomb); #endif #endif /* _@GUARD_PREFIX@_STDLIB_H */ #endif /* _@GUARD_PREFIX@_STDLIB_H */ #endif gnuastro-0.5/bootstrapped/lib/stdio.in.h0000644000175000017500000014437113217200021015313 00000000000000/* A GNU-like . Copyright (C) 2004, 2007-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_FILE || defined __need___FILE || defined _GL_ALREADY_INCLUDING_STDIO_H /* Special invocation convention: - Inside glibc header files. - On OSF/1 5.1 we have a sequence of nested includes -> -> -> -> -> -> -> . In this situation, the functions are not yet declared, therefore we cannot provide the C++ aliases. */ #@INCLUDE_NEXT@ @NEXT_STDIO_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_STDIO_H #define _GL_ALREADY_INCLUDING_STDIO_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_STDIO_H@ #undef _GL_ALREADY_INCLUDING_STDIO_H #ifndef _@GUARD_PREFIX@_STDIO_H #define _@GUARD_PREFIX@_STDIO_H /* Get va_list. Needed on many systems, including glibc 2.8. */ #include #include /* Get off_t and ssize_t. Needed on many systems, including glibc 2.8 and eglibc 2.11.2. May also define off_t to a 64-bit type on native Windows. */ #include /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif /* _GL_ATTRIBUTE_FORMAT_PRINTF indicates to GCC that the function takes a format string and arguments, where the format string directives are the ones standardized by ISO C99 and POSIX. */ #if __GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4) # define _GL_ATTRIBUTE_FORMAT_PRINTF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__gnu_printf__, formatstring_parameter, first_argument)) #else # define _GL_ATTRIBUTE_FORMAT_PRINTF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__printf__, formatstring_parameter, first_argument)) #endif /* _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM is like _GL_ATTRIBUTE_FORMAT_PRINTF, except that it indicates to GCC that the supported format string directives are the ones of the system printf(), rather than the ones standardized by ISO C99 and POSIX. */ #if GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU # define _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT_PRINTF (formatstring_parameter, first_argument) #else # define _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__printf__, formatstring_parameter, first_argument)) #endif /* _GL_ATTRIBUTE_FORMAT_SCANF indicates to GCC that the function takes a format string and arguments, where the format string directives are the ones standardized by ISO C99 and POSIX. */ #if __GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4) # define _GL_ATTRIBUTE_FORMAT_SCANF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__gnu_scanf__, formatstring_parameter, first_argument)) #else # define _GL_ATTRIBUTE_FORMAT_SCANF(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__scanf__, formatstring_parameter, first_argument)) #endif /* _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM is like _GL_ATTRIBUTE_FORMAT_SCANF, except that it indicates to GCC that the supported format string directives are the ones of the system scanf(), rather than the ones standardized by ISO C99 and POSIX. */ #define _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM(formatstring_parameter, first_argument) \ _GL_ATTRIBUTE_FORMAT ((__scanf__, formatstring_parameter, first_argument)) /* Solaris 10 and NetBSD 7.0 declare renameat in , not in . */ /* But in any case avoid namespace pollution on glibc systems. */ #if (@GNULIB_RENAMEAT@ || defined GNULIB_POSIXCHECK) && (defined __sun || defined __NetBSD__) \ && ! defined __GLIBC__ # include #endif /* MSVC declares 'perror' in , not in . We must include it before we #define perror rpl_perror. */ /* But in any case avoid namespace pollution on glibc systems. */ #if (@GNULIB_PERROR@ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) \ && ! defined __GLIBC__ # include #endif /* MSVC declares 'remove' in , not in . We must include it before we #define remove rpl_remove. */ /* MSVC declares 'rename' in , not in . We must include it before we #define rename rpl_rename. */ /* But in any case avoid namespace pollution on glibc systems. */ #if (@GNULIB_REMOVE@ || @GNULIB_RENAME@ || defined GNULIB_POSIXCHECK) \ && ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) \ && ! defined __GLIBC__ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Macros for stringification. */ #define _GL_STDIO_STRINGIZE(token) #token #define _GL_STDIO_MACROEXPAND_AND_STRINGIZE(token) _GL_STDIO_STRINGIZE(token) /* When also using extern inline, suppress the use of static inline in standard headers of problematic Apple configurations, as Libc at least through Libc-825.26 (2013-04-09) mishandles it; see, e.g., . Perhaps Apple will fix this some day. */ #if (defined _GL_EXTERN_INLINE_IN_USE && defined __APPLE__ \ && defined __GNUC__ && defined __STDC__) # undef putc_unlocked #endif #if @GNULIB_DPRINTF@ # if @REPLACE_DPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define dprintf rpl_dprintf # endif _GL_FUNCDECL_RPL (dprintf, int, (int fd, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (dprintf, int, (int fd, const char *format, ...)); # else # if !@HAVE_DPRINTF@ _GL_FUNCDECL_SYS (dprintf, int, (int fd, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (dprintf, int, (int fd, const char *format, ...)); # endif _GL_CXXALIASWARN (dprintf); #elif defined GNULIB_POSIXCHECK # undef dprintf # if HAVE_RAW_DECL_DPRINTF _GL_WARN_ON_USE (dprintf, "dprintf is unportable - " "use gnulib module dprintf for portability"); # endif #endif #if @GNULIB_FCLOSE@ /* Close STREAM and its underlying file descriptor. */ # if @REPLACE_FCLOSE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fclose rpl_fclose # endif _GL_FUNCDECL_RPL (fclose, int, (FILE *stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fclose, int, (FILE *stream)); # else _GL_CXXALIAS_SYS (fclose, int, (FILE *stream)); # endif _GL_CXXALIASWARN (fclose); #elif defined GNULIB_POSIXCHECK # undef fclose /* Assume fclose is always declared. */ _GL_WARN_ON_USE (fclose, "fclose is not always POSIX compliant - " "use gnulib module fclose for portable POSIX compliance"); #endif #if @GNULIB_FDOPEN@ # if @REPLACE_FDOPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fdopen # define fdopen rpl_fdopen # endif _GL_FUNCDECL_RPL (fdopen, FILE *, (int fd, const char *mode) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fdopen, FILE *, (int fd, const char *mode)); # else _GL_CXXALIAS_SYS (fdopen, FILE *, (int fd, const char *mode)); # endif _GL_CXXALIASWARN (fdopen); #elif defined GNULIB_POSIXCHECK # undef fdopen /* Assume fdopen is always declared. */ _GL_WARN_ON_USE (fdopen, "fdopen on native Windows platforms is not POSIX compliant - " "use gnulib module fdopen for portability"); #endif #if @GNULIB_FFLUSH@ /* Flush all pending data on STREAM according to POSIX rules. Both output and seekable input streams are supported. Note! LOSS OF DATA can occur if fflush is applied on an input stream that is _not_seekable_ or on an update stream that is _not_seekable_ and in which the most recent operation was input. Seekability can be tested with lseek(fileno(fp),0,SEEK_CUR). */ # if @REPLACE_FFLUSH@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fflush rpl_fflush # endif _GL_FUNCDECL_RPL (fflush, int, (FILE *gl_stream)); _GL_CXXALIAS_RPL (fflush, int, (FILE *gl_stream)); # else _GL_CXXALIAS_SYS (fflush, int, (FILE *gl_stream)); # endif _GL_CXXALIASWARN (fflush); #elif defined GNULIB_POSIXCHECK # undef fflush /* Assume fflush is always declared. */ _GL_WARN_ON_USE (fflush, "fflush is not always POSIX compliant - " "use gnulib module fflush for portable POSIX compliance"); #endif #if @GNULIB_FGETC@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fgetc # define fgetc rpl_fgetc # endif _GL_FUNCDECL_RPL (fgetc, int, (FILE *stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fgetc, int, (FILE *stream)); # else _GL_CXXALIAS_SYS (fgetc, int, (FILE *stream)); # endif _GL_CXXALIASWARN (fgetc); #endif #if @GNULIB_FGETS@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fgets # define fgets rpl_fgets # endif _GL_FUNCDECL_RPL (fgets, char *, (char *s, int n, FILE *stream) _GL_ARG_NONNULL ((1, 3))); _GL_CXXALIAS_RPL (fgets, char *, (char *s, int n, FILE *stream)); # else _GL_CXXALIAS_SYS (fgets, char *, (char *s, int n, FILE *stream)); # endif _GL_CXXALIASWARN (fgets); #endif #if @GNULIB_FOPEN@ # if @REPLACE_FOPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fopen # define fopen rpl_fopen # endif _GL_FUNCDECL_RPL (fopen, FILE *, (const char *filename, const char *mode) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (fopen, FILE *, (const char *filename, const char *mode)); # else _GL_CXXALIAS_SYS (fopen, FILE *, (const char *filename, const char *mode)); # endif _GL_CXXALIASWARN (fopen); #elif defined GNULIB_POSIXCHECK # undef fopen /* Assume fopen is always declared. */ _GL_WARN_ON_USE (fopen, "fopen on native Windows platforms is not POSIX compliant - " "use gnulib module fopen for portability"); #endif #if @GNULIB_FPRINTF_POSIX@ || @GNULIB_FPRINTF@ # if (@GNULIB_FPRINTF_POSIX@ && @REPLACE_FPRINTF@) \ || (@GNULIB_FPRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fprintf rpl_fprintf # endif # define GNULIB_overrides_fprintf 1 # if @GNULIB_FPRINTF_POSIX@ || @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL (fprintf, int, (FILE *fp, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); # else _GL_FUNCDECL_RPL (fprintf, int, (FILE *fp, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (2, 3) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_RPL (fprintf, int, (FILE *fp, const char *format, ...)); # else _GL_CXXALIAS_SYS (fprintf, int, (FILE *fp, const char *format, ...)); # endif _GL_CXXALIASWARN (fprintf); #endif #if !@GNULIB_FPRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_fprintf # undef fprintf # endif /* Assume fprintf is always declared. */ _GL_WARN_ON_USE (fprintf, "fprintf is not always POSIX compliant - " "use gnulib module fprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_FPURGE@ /* Discard all pending buffered I/O data on STREAM. STREAM must not be wide-character oriented. When discarding pending output, the file position is set back to where it was before the write calls. When discarding pending input, the file position is advanced to match the end of the previously read input. Return 0 if successful. Upon error, return -1 and set errno. */ # if @REPLACE_FPURGE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define fpurge rpl_fpurge # endif _GL_FUNCDECL_RPL (fpurge, int, (FILE *gl_stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fpurge, int, (FILE *gl_stream)); # else # if !@HAVE_DECL_FPURGE@ _GL_FUNCDECL_SYS (fpurge, int, (FILE *gl_stream) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (fpurge, int, (FILE *gl_stream)); # endif _GL_CXXALIASWARN (fpurge); #elif defined GNULIB_POSIXCHECK # undef fpurge # if HAVE_RAW_DECL_FPURGE _GL_WARN_ON_USE (fpurge, "fpurge is not always present - " "use gnulib module fpurge for portability"); # endif #endif #if @GNULIB_FPUTC@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fputc # define fputc rpl_fputc # endif _GL_FUNCDECL_RPL (fputc, int, (int c, FILE *stream) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (fputc, int, (int c, FILE *stream)); # else _GL_CXXALIAS_SYS (fputc, int, (int c, FILE *stream)); # endif _GL_CXXALIASWARN (fputc); #endif #if @GNULIB_FPUTS@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fputs # define fputs rpl_fputs # endif _GL_FUNCDECL_RPL (fputs, int, (const char *string, FILE *stream) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (fputs, int, (const char *string, FILE *stream)); # else _GL_CXXALIAS_SYS (fputs, int, (const char *string, FILE *stream)); # endif _GL_CXXALIASWARN (fputs); #endif #if @GNULIB_FREAD@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fread # define fread rpl_fread # endif _GL_FUNCDECL_RPL (fread, size_t, (void *ptr, size_t s, size_t n, FILE *stream) _GL_ARG_NONNULL ((4))); _GL_CXXALIAS_RPL (fread, size_t, (void *ptr, size_t s, size_t n, FILE *stream)); # else _GL_CXXALIAS_SYS (fread, size_t, (void *ptr, size_t s, size_t n, FILE *stream)); # endif _GL_CXXALIASWARN (fread); #endif #if @GNULIB_FREOPEN@ # if @REPLACE_FREOPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef freopen # define freopen rpl_freopen # endif _GL_FUNCDECL_RPL (freopen, FILE *, (const char *filename, const char *mode, FILE *stream) _GL_ARG_NONNULL ((2, 3))); _GL_CXXALIAS_RPL (freopen, FILE *, (const char *filename, const char *mode, FILE *stream)); # else _GL_CXXALIAS_SYS (freopen, FILE *, (const char *filename, const char *mode, FILE *stream)); # endif _GL_CXXALIASWARN (freopen); #elif defined GNULIB_POSIXCHECK # undef freopen /* Assume freopen is always declared. */ _GL_WARN_ON_USE (freopen, "freopen on native Windows platforms is not POSIX compliant - " "use gnulib module freopen for portability"); #endif #if @GNULIB_FSCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fscanf # define fscanf rpl_fscanf # endif _GL_FUNCDECL_RPL (fscanf, int, (FILE *stream, const char *format, ...) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (fscanf, int, (FILE *stream, const char *format, ...)); # else _GL_CXXALIAS_SYS (fscanf, int, (FILE *stream, const char *format, ...)); # endif _GL_CXXALIASWARN (fscanf); #endif /* Set up the following warnings, based on which modules are in use. GNU Coding Standards discourage the use of fseek, since it imposes an arbitrary limitation on some 32-bit hosts. Remember that the fseek module depends on the fseeko module, so we only have three cases to consider: 1. The developer is not using either module. Issue a warning under GNULIB_POSIXCHECK for both functions, to remind them that both functions have bugs on some systems. _GL_NO_LARGE_FILES has no impact on this warning. 2. The developer is using both modules. They may be unaware of the arbitrary limitations of fseek, so issue a warning under GNULIB_POSIXCHECK. On the other hand, they may be using both modules intentionally, so the developer can define _GL_NO_LARGE_FILES in the compilation units where the use of fseek is safe, to silence the warning. 3. The developer is using the fseeko module, but not fseek. Gnulib guarantees that fseek will still work around platform bugs in that case, but we presume that the developer is aware of the pitfalls of fseek and was trying to avoid it, so issue a warning even when GNULIB_POSIXCHECK is undefined. Again, _GL_NO_LARGE_FILES can be defined to silence the warning in particular compilation units. In C++ compilations with GNULIB_NAMESPACE, in order to avoid that fseek gets defined as a macro, it is recommended that the developer uses the fseek module, even if he is not calling the fseek function. Most gnulib clients that perform stream operations should fall into category 3. */ #if @GNULIB_FSEEK@ # if defined GNULIB_POSIXCHECK && !defined _GL_NO_LARGE_FILES # define _GL_FSEEK_WARN /* Category 2, above. */ # undef fseek # endif # if @REPLACE_FSEEK@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fseek # define fseek rpl_fseek # endif _GL_FUNCDECL_RPL (fseek, int, (FILE *fp, long offset, int whence) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fseek, int, (FILE *fp, long offset, int whence)); # else _GL_CXXALIAS_SYS (fseek, int, (FILE *fp, long offset, int whence)); # endif _GL_CXXALIASWARN (fseek); #endif #if @GNULIB_FSEEKO@ # if !@GNULIB_FSEEK@ && !defined _GL_NO_LARGE_FILES # define _GL_FSEEK_WARN /* Category 3, above. */ # undef fseek # endif # if @REPLACE_FSEEKO@ /* Provide an fseeko function that is aware of a preceding fflush(), and which detects pipes. */ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fseeko # define fseeko rpl_fseeko # endif _GL_FUNCDECL_RPL (fseeko, int, (FILE *fp, off_t offset, int whence) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (fseeko, int, (FILE *fp, off_t offset, int whence)); # else # if ! @HAVE_DECL_FSEEKO@ _GL_FUNCDECL_SYS (fseeko, int, (FILE *fp, off_t offset, int whence) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (fseeko, int, (FILE *fp, off_t offset, int whence)); # endif _GL_CXXALIASWARN (fseeko); #elif defined GNULIB_POSIXCHECK # define _GL_FSEEK_WARN /* Category 1, above. */ # undef fseek # undef fseeko # if HAVE_RAW_DECL_FSEEKO _GL_WARN_ON_USE (fseeko, "fseeko is unportable - " "use gnulib module fseeko for portability"); # endif #endif #ifdef _GL_FSEEK_WARN # undef _GL_FSEEK_WARN /* Here, either fseek is undefined (but C89 guarantees that it is declared), or it is defined as rpl_fseek (declared above). */ _GL_WARN_ON_USE (fseek, "fseek cannot handle files larger than 4 GB " "on 32-bit platforms - " "use fseeko function for handling of large files"); #endif /* ftell, ftello. See the comments on fseek/fseeko. */ #if @GNULIB_FTELL@ # if defined GNULIB_POSIXCHECK && !defined _GL_NO_LARGE_FILES # define _GL_FTELL_WARN /* Category 2, above. */ # undef ftell # endif # if @REPLACE_FTELL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ftell # define ftell rpl_ftell # endif _GL_FUNCDECL_RPL (ftell, long, (FILE *fp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (ftell, long, (FILE *fp)); # else _GL_CXXALIAS_SYS (ftell, long, (FILE *fp)); # endif _GL_CXXALIASWARN (ftell); #endif #if @GNULIB_FTELLO@ # if !@GNULIB_FTELL@ && !defined _GL_NO_LARGE_FILES # define _GL_FTELL_WARN /* Category 3, above. */ # undef ftell # endif # if @REPLACE_FTELLO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ftello # define ftello rpl_ftello # endif _GL_FUNCDECL_RPL (ftello, off_t, (FILE *fp) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (ftello, off_t, (FILE *fp)); # else # if ! @HAVE_DECL_FTELLO@ _GL_FUNCDECL_SYS (ftello, off_t, (FILE *fp) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (ftello, off_t, (FILE *fp)); # endif _GL_CXXALIASWARN (ftello); #elif defined GNULIB_POSIXCHECK # define _GL_FTELL_WARN /* Category 1, above. */ # undef ftell # undef ftello # if HAVE_RAW_DECL_FTELLO _GL_WARN_ON_USE (ftello, "ftello is unportable - " "use gnulib module ftello for portability"); # endif #endif #ifdef _GL_FTELL_WARN # undef _GL_FTELL_WARN /* Here, either ftell is undefined (but C89 guarantees that it is declared), or it is defined as rpl_ftell (declared above). */ _GL_WARN_ON_USE (ftell, "ftell cannot handle files larger than 4 GB " "on 32-bit platforms - " "use ftello function for handling of large files"); #endif #if @GNULIB_FWRITE@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fwrite # define fwrite rpl_fwrite # endif _GL_FUNCDECL_RPL (fwrite, size_t, (const void *ptr, size_t s, size_t n, FILE *stream) _GL_ARG_NONNULL ((1, 4))); _GL_CXXALIAS_RPL (fwrite, size_t, (const void *ptr, size_t s, size_t n, FILE *stream)); # else _GL_CXXALIAS_SYS (fwrite, size_t, (const void *ptr, size_t s, size_t n, FILE *stream)); /* Work around bug 11959 when fortifying glibc 2.4 through 2.15 , which sometimes causes an unwanted diagnostic for fwrite calls. This affects only function declaration attributes under certain versions of gcc and clang, and is not needed for C++. */ # if (0 < __USE_FORTIFY_LEVEL \ && __GLIBC__ == 2 && 4 <= __GLIBC_MINOR__ && __GLIBC_MINOR__ <= 15 \ && 3 < __GNUC__ + (4 <= __GNUC_MINOR__) \ && !defined __cplusplus) # undef fwrite # undef fwrite_unlocked extern size_t __REDIRECT (rpl_fwrite, (const void *__restrict, size_t, size_t, FILE *__restrict), fwrite); extern size_t __REDIRECT (rpl_fwrite_unlocked, (const void *__restrict, size_t, size_t, FILE *__restrict), fwrite_unlocked); # define fwrite rpl_fwrite # define fwrite_unlocked rpl_fwrite_unlocked # endif # endif _GL_CXXALIASWARN (fwrite); #endif #if @GNULIB_GETC@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getc # define getc rpl_fgetc # endif _GL_FUNCDECL_RPL (fgetc, int, (FILE *stream) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL_1 (getc, rpl_fgetc, int, (FILE *stream)); # else _GL_CXXALIAS_SYS (getc, int, (FILE *stream)); # endif _GL_CXXALIASWARN (getc); #endif #if @GNULIB_GETCHAR@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getchar # define getchar rpl_getchar # endif _GL_FUNCDECL_RPL (getchar, int, (void)); _GL_CXXALIAS_RPL (getchar, int, (void)); # else _GL_CXXALIAS_SYS (getchar, int, (void)); # endif _GL_CXXALIASWARN (getchar); #endif #if @GNULIB_GETDELIM@ /* Read input, up to (and including) the next occurrence of DELIMITER, from STREAM, store it in *LINEPTR (and NUL-terminate it). *LINEPTR is a pointer returned from malloc (or NULL), pointing to *LINESIZE bytes of space. It is realloc'd as necessary. Return the number of bytes read and stored at *LINEPTR (not including the NUL terminator), or -1 on error or EOF. */ # if @REPLACE_GETDELIM@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getdelim # define getdelim rpl_getdelim # endif _GL_FUNCDECL_RPL (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream) _GL_ARG_NONNULL ((1, 2, 4))); _GL_CXXALIAS_RPL (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream)); # else # if !@HAVE_DECL_GETDELIM@ _GL_FUNCDECL_SYS (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream) _GL_ARG_NONNULL ((1, 2, 4))); # endif _GL_CXXALIAS_SYS (getdelim, ssize_t, (char **lineptr, size_t *linesize, int delimiter, FILE *stream)); # endif _GL_CXXALIASWARN (getdelim); #elif defined GNULIB_POSIXCHECK # undef getdelim # if HAVE_RAW_DECL_GETDELIM _GL_WARN_ON_USE (getdelim, "getdelim is unportable - " "use gnulib module getdelim for portability"); # endif #endif #if @GNULIB_GETLINE@ /* Read a line, up to (and including) the next newline, from STREAM, store it in *LINEPTR (and NUL-terminate it). *LINEPTR is a pointer returned from malloc (or NULL), pointing to *LINESIZE bytes of space. It is realloc'd as necessary. Return the number of bytes read and stored at *LINEPTR (not including the NUL terminator), or -1 on error or EOF. */ # if @REPLACE_GETLINE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef getline # define getline rpl_getline # endif _GL_FUNCDECL_RPL (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream) _GL_ARG_NONNULL ((1, 2, 3))); _GL_CXXALIAS_RPL (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream)); # else # if !@HAVE_DECL_GETLINE@ _GL_FUNCDECL_SYS (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream) _GL_ARG_NONNULL ((1, 2, 3))); # endif _GL_CXXALIAS_SYS (getline, ssize_t, (char **lineptr, size_t *linesize, FILE *stream)); # endif # if @HAVE_DECL_GETLINE@ _GL_CXXALIASWARN (getline); # endif #elif defined GNULIB_POSIXCHECK # undef getline # if HAVE_RAW_DECL_GETLINE _GL_WARN_ON_USE (getline, "getline is unportable - " "use gnulib module getline for portability"); # endif #endif /* It is very rare that the developer ever has full control of stdin, so any use of gets warrants an unconditional warning; besides, C11 removed it. */ #undef gets #if HAVE_RAW_DECL_GETS && !defined __cplusplus _GL_WARN_ON_USE (gets, "gets is a security hole - use fgets instead"); #endif #if @GNULIB_OBSTACK_PRINTF@ || @GNULIB_OBSTACK_PRINTF_POSIX@ struct obstack; /* Grow an obstack with formatted output. Return the number of bytes added to OBS. No trailing nul byte is added, and the object should be closed with obstack_finish before use. Upon memory allocation error, call obstack_alloc_failed_handler. Upon other error, return -1. */ # if @REPLACE_OBSTACK_PRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define obstack_printf rpl_obstack_printf # endif _GL_FUNCDECL_RPL (obstack_printf, int, (struct obstack *obs, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (obstack_printf, int, (struct obstack *obs, const char *format, ...)); # else # if !@HAVE_DECL_OBSTACK_PRINTF@ _GL_FUNCDECL_SYS (obstack_printf, int, (struct obstack *obs, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (obstack_printf, int, (struct obstack *obs, const char *format, ...)); # endif _GL_CXXALIASWARN (obstack_printf); # if @REPLACE_OBSTACK_PRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define obstack_vprintf rpl_obstack_vprintf # endif _GL_FUNCDECL_RPL (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args)); # else # if !@HAVE_DECL_OBSTACK_PRINTF@ _GL_FUNCDECL_SYS (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (obstack_vprintf, int, (struct obstack *obs, const char *format, va_list args)); # endif _GL_CXXALIASWARN (obstack_vprintf); #endif #if @GNULIB_PCLOSE@ # if !@HAVE_PCLOSE@ _GL_FUNCDECL_SYS (pclose, int, (FILE *stream) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (pclose, int, (FILE *stream)); _GL_CXXALIASWARN (pclose); #elif defined GNULIB_POSIXCHECK # undef pclose # if HAVE_RAW_DECL_PCLOSE _GL_WARN_ON_USE (pclose, "pclose is unportable - " "use gnulib module pclose for more portability"); # endif #endif #if @GNULIB_PERROR@ /* Print a message to standard error, describing the value of ERRNO, (if STRING is not NULL and not empty) prefixed with STRING and ": ", and terminated with a newline. */ # if @REPLACE_PERROR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define perror rpl_perror # endif _GL_FUNCDECL_RPL (perror, void, (const char *string)); _GL_CXXALIAS_RPL (perror, void, (const char *string)); # else _GL_CXXALIAS_SYS (perror, void, (const char *string)); # endif _GL_CXXALIASWARN (perror); #elif defined GNULIB_POSIXCHECK # undef perror /* Assume perror is always declared. */ _GL_WARN_ON_USE (perror, "perror is not always POSIX compliant - " "use gnulib module perror for portability"); #endif #if @GNULIB_POPEN@ # if @REPLACE_POPEN@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef popen # define popen rpl_popen # endif _GL_FUNCDECL_RPL (popen, FILE *, (const char *cmd, const char *mode) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (popen, FILE *, (const char *cmd, const char *mode)); # else # if !@HAVE_POPEN@ _GL_FUNCDECL_SYS (popen, FILE *, (const char *cmd, const char *mode) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (popen, FILE *, (const char *cmd, const char *mode)); # endif _GL_CXXALIASWARN (popen); #elif defined GNULIB_POSIXCHECK # undef popen # if HAVE_RAW_DECL_POPEN _GL_WARN_ON_USE (popen, "popen is buggy on some platforms - " "use gnulib module popen or pipe for more portability"); # endif #endif #if @GNULIB_PRINTF_POSIX@ || @GNULIB_PRINTF@ # if (@GNULIB_PRINTF_POSIX@ && @REPLACE_PRINTF@) \ || (@GNULIB_PRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if defined __GNUC__ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) /* Don't break __attribute__((format(printf,M,N))). */ # define printf __printf__ # endif # if @GNULIB_PRINTF_POSIX@ || @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL_1 (__printf__, int, (const char *format, ...) __asm__ (@ASM_SYMBOL_PREFIX@ _GL_STDIO_MACROEXPAND_AND_STRINGIZE(rpl_printf)) _GL_ATTRIBUTE_FORMAT_PRINTF (1, 2) _GL_ARG_NONNULL ((1))); # else _GL_FUNCDECL_RPL_1 (__printf__, int, (const char *format, ...) __asm__ (@ASM_SYMBOL_PREFIX@ _GL_STDIO_MACROEXPAND_AND_STRINGIZE(rpl_printf)) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (1, 2) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_RPL_1 (printf, __printf__, int, (const char *format, ...)); # else # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define printf rpl_printf # endif _GL_FUNCDECL_RPL (printf, int, (const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (1, 2) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (printf, int, (const char *format, ...)); # endif # define GNULIB_overrides_printf 1 # else _GL_CXXALIAS_SYS (printf, int, (const char *format, ...)); # endif _GL_CXXALIASWARN (printf); #endif #if !@GNULIB_PRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_printf # undef printf # endif /* Assume printf is always declared. */ _GL_WARN_ON_USE (printf, "printf is not always POSIX compliant - " "use gnulib module printf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_PUTC@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef putc # define putc rpl_fputc # endif _GL_FUNCDECL_RPL (fputc, int, (int c, FILE *stream) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL_1 (putc, rpl_fputc, int, (int c, FILE *stream)); # else _GL_CXXALIAS_SYS (putc, int, (int c, FILE *stream)); # endif _GL_CXXALIASWARN (putc); #endif #if @GNULIB_PUTCHAR@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef putchar # define putchar rpl_putchar # endif _GL_FUNCDECL_RPL (putchar, int, (int c)); _GL_CXXALIAS_RPL (putchar, int, (int c)); # else _GL_CXXALIAS_SYS (putchar, int, (int c)); # endif _GL_CXXALIASWARN (putchar); #endif #if @GNULIB_PUTS@ # if @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef puts # define puts rpl_puts # endif _GL_FUNCDECL_RPL (puts, int, (const char *string) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (puts, int, (const char *string)); # else _GL_CXXALIAS_SYS (puts, int, (const char *string)); # endif _GL_CXXALIASWARN (puts); #endif #if @GNULIB_REMOVE@ # if @REPLACE_REMOVE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remove # define remove rpl_remove # endif _GL_FUNCDECL_RPL (remove, int, (const char *name) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (remove, int, (const char *name)); # else _GL_CXXALIAS_SYS (remove, int, (const char *name)); # endif _GL_CXXALIASWARN (remove); #elif defined GNULIB_POSIXCHECK # undef remove /* Assume remove is always declared. */ _GL_WARN_ON_USE (remove, "remove cannot handle directories on some platforms - " "use gnulib module remove for more portability"); #endif #if @GNULIB_RENAME@ # if @REPLACE_RENAME@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef rename # define rename rpl_rename # endif _GL_FUNCDECL_RPL (rename, int, (const char *old_filename, const char *new_filename) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (rename, int, (const char *old_filename, const char *new_filename)); # else _GL_CXXALIAS_SYS (rename, int, (const char *old_filename, const char *new_filename)); # endif _GL_CXXALIASWARN (rename); #elif defined GNULIB_POSIXCHECK # undef rename /* Assume rename is always declared. */ _GL_WARN_ON_USE (rename, "rename is buggy on some platforms - " "use gnulib module rename for more portability"); #endif #if @GNULIB_RENAMEAT@ # if @REPLACE_RENAMEAT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef renameat # define renameat rpl_renameat # endif _GL_FUNCDECL_RPL (renameat, int, (int fd1, char const *file1, int fd2, char const *file2) _GL_ARG_NONNULL ((2, 4))); _GL_CXXALIAS_RPL (renameat, int, (int fd1, char const *file1, int fd2, char const *file2)); # else # if !@HAVE_RENAMEAT@ _GL_FUNCDECL_SYS (renameat, int, (int fd1, char const *file1, int fd2, char const *file2) _GL_ARG_NONNULL ((2, 4))); # endif _GL_CXXALIAS_SYS (renameat, int, (int fd1, char const *file1, int fd2, char const *file2)); # endif _GL_CXXALIASWARN (renameat); #elif defined GNULIB_POSIXCHECK # undef renameat # if HAVE_RAW_DECL_RENAMEAT _GL_WARN_ON_USE (renameat, "renameat is not portable - " "use gnulib module renameat for portability"); # endif #endif #if @GNULIB_SCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if defined __GNUC__ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef scanf /* Don't break __attribute__((format(scanf,M,N))). */ # define scanf __scanf__ # endif _GL_FUNCDECL_RPL_1 (__scanf__, int, (const char *format, ...) __asm__ (@ASM_SYMBOL_PREFIX@ _GL_STDIO_MACROEXPAND_AND_STRINGIZE(rpl_scanf)) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (1, 2) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL_1 (scanf, __scanf__, int, (const char *format, ...)); # else # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef scanf # define scanf rpl_scanf # endif _GL_FUNCDECL_RPL (scanf, int, (const char *format, ...) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (1, 2) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (scanf, int, (const char *format, ...)); # endif # else _GL_CXXALIAS_SYS (scanf, int, (const char *format, ...)); # endif _GL_CXXALIASWARN (scanf); #endif #if @GNULIB_SNPRINTF@ # if @REPLACE_SNPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define snprintf rpl_snprintf # endif _GL_FUNCDECL_RPL (snprintf, int, (char *str, size_t size, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 4) _GL_ARG_NONNULL ((3))); _GL_CXXALIAS_RPL (snprintf, int, (char *str, size_t size, const char *format, ...)); # else # if !@HAVE_DECL_SNPRINTF@ _GL_FUNCDECL_SYS (snprintf, int, (char *str, size_t size, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 4) _GL_ARG_NONNULL ((3))); # endif _GL_CXXALIAS_SYS (snprintf, int, (char *str, size_t size, const char *format, ...)); # endif _GL_CXXALIASWARN (snprintf); #elif defined GNULIB_POSIXCHECK # undef snprintf # if HAVE_RAW_DECL_SNPRINTF _GL_WARN_ON_USE (snprintf, "snprintf is unportable - " "use gnulib module snprintf for portability"); # endif #endif /* Some people would argue that all sprintf uses should be warned about (for example, OpenBSD issues a link warning for it), since it can cause security holes due to buffer overruns. However, we believe that sprintf can be used safely, and is more efficient than snprintf in those safe cases; and as proof of our belief, we use sprintf in several gnulib modules. So this header intentionally avoids adding a warning to sprintf except when GNULIB_POSIXCHECK is defined. */ #if @GNULIB_SPRINTF_POSIX@ # if @REPLACE_SPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define sprintf rpl_sprintf # endif _GL_FUNCDECL_RPL (sprintf, int, (char *str, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (sprintf, int, (char *str, const char *format, ...)); # else _GL_CXXALIAS_SYS (sprintf, int, (char *str, const char *format, ...)); # endif _GL_CXXALIASWARN (sprintf); #elif defined GNULIB_POSIXCHECK # undef sprintf /* Assume sprintf is always declared. */ _GL_WARN_ON_USE (sprintf, "sprintf is not always POSIX compliant - " "use gnulib module sprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_TMPFILE@ # if @REPLACE_TMPFILE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define tmpfile rpl_tmpfile # endif _GL_FUNCDECL_RPL (tmpfile, FILE *, (void)); _GL_CXXALIAS_RPL (tmpfile, FILE *, (void)); # else _GL_CXXALIAS_SYS (tmpfile, FILE *, (void)); # endif _GL_CXXALIASWARN (tmpfile); #elif defined GNULIB_POSIXCHECK # undef tmpfile # if HAVE_RAW_DECL_TMPFILE _GL_WARN_ON_USE (tmpfile, "tmpfile is not usable on mingw - " "use gnulib module tmpfile for portability"); # endif #endif #if @GNULIB_VASPRINTF@ /* Write formatted output to a string dynamically allocated with malloc(). If the memory allocation succeeds, store the address of the string in *RESULT and return the number of resulting bytes, excluding the trailing NUL. Upon memory allocation error, or some other error, return -1. */ # if @REPLACE_VASPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define asprintf rpl_asprintf # endif _GL_FUNCDECL_RPL (asprintf, int, (char **result, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (asprintf, int, (char **result, const char *format, ...)); # else # if !@HAVE_VASPRINTF@ _GL_FUNCDECL_SYS (asprintf, int, (char **result, const char *format, ...) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 3) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (asprintf, int, (char **result, const char *format, ...)); # endif _GL_CXXALIASWARN (asprintf); # if @REPLACE_VASPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vasprintf rpl_vasprintf # endif _GL_FUNCDECL_RPL (vasprintf, int, (char **result, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (vasprintf, int, (char **result, const char *format, va_list args)); # else # if !@HAVE_VASPRINTF@ _GL_FUNCDECL_SYS (vasprintf, int, (char **result, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_SYS (vasprintf, int, (char **result, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vasprintf); #endif #if @GNULIB_VDPRINTF@ # if @REPLACE_VDPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vdprintf rpl_vdprintf # endif _GL_FUNCDECL_RPL (vdprintf, int, (int fd, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (vdprintf, int, (int fd, const char *format, va_list args)); # else # if !@HAVE_VDPRINTF@ _GL_FUNCDECL_SYS (vdprintf, int, (int fd, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((2))); # endif /* Need to cast, because on Solaris, the third parameter will likely be __va_list args. */ _GL_CXXALIAS_SYS_CAST (vdprintf, int, (int fd, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vdprintf); #elif defined GNULIB_POSIXCHECK # undef vdprintf # if HAVE_RAW_DECL_VDPRINTF _GL_WARN_ON_USE (vdprintf, "vdprintf is unportable - " "use gnulib module vdprintf for portability"); # endif #endif #if @GNULIB_VFPRINTF_POSIX@ || @GNULIB_VFPRINTF@ # if (@GNULIB_VFPRINTF_POSIX@ && @REPLACE_VFPRINTF@) \ || (@GNULIB_VFPRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vfprintf rpl_vfprintf # endif # define GNULIB_overrides_vfprintf 1 # if @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL (vfprintf, int, (FILE *fp, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); # else _GL_FUNCDECL_RPL (vfprintf, int, (FILE *fp, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (2, 0) _GL_ARG_NONNULL ((1, 2))); # endif _GL_CXXALIAS_RPL (vfprintf, int, (FILE *fp, const char *format, va_list args)); # else /* Need to cast, because on Solaris, the third parameter is __va_list args and GCC's fixincludes did not change this to __gnuc_va_list. */ _GL_CXXALIAS_SYS_CAST (vfprintf, int, (FILE *fp, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vfprintf); #endif #if !@GNULIB_VFPRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_vfprintf # undef vfprintf # endif /* Assume vfprintf is always declared. */ _GL_WARN_ON_USE (vfprintf, "vfprintf is not always POSIX compliant - " "use gnulib module vfprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_VFSCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef vfscanf # define vfscanf rpl_vfscanf # endif _GL_FUNCDECL_RPL (vfscanf, int, (FILE *stream, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (vfscanf, int, (FILE *stream, const char *format, va_list args)); # else _GL_CXXALIAS_SYS (vfscanf, int, (FILE *stream, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vfscanf); #endif #if @GNULIB_VPRINTF_POSIX@ || @GNULIB_VPRINTF@ # if (@GNULIB_VPRINTF_POSIX@ && @REPLACE_VPRINTF@) \ || (@GNULIB_VPRINTF@ && @REPLACE_STDIO_WRITE_FUNCS@ && (@GNULIB_STDIO_H_NONBLOCKING@ || @GNULIB_STDIO_H_SIGPIPE@)) # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vprintf rpl_vprintf # endif # define GNULIB_overrides_vprintf 1 # if @GNULIB_VPRINTF_POSIX@ || @GNULIB_VFPRINTF_POSIX@ _GL_FUNCDECL_RPL (vprintf, int, (const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (1, 0) _GL_ARG_NONNULL ((1))); # else _GL_FUNCDECL_RPL (vprintf, int, (const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF_SYSTEM (1, 0) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_RPL (vprintf, int, (const char *format, va_list args)); # else /* Need to cast, because on Solaris, the second parameter is __va_list args and GCC's fixincludes did not change this to __gnuc_va_list. */ _GL_CXXALIAS_SYS_CAST (vprintf, int, (const char *format, va_list args)); # endif _GL_CXXALIASWARN (vprintf); #endif #if !@GNULIB_VPRINTF_POSIX@ && defined GNULIB_POSIXCHECK # if !GNULIB_overrides_vprintf # undef vprintf # endif /* Assume vprintf is always declared. */ _GL_WARN_ON_USE (vprintf, "vprintf is not always POSIX compliant - " "use gnulib module vprintf-posix for portable " "POSIX compliance"); #endif #if @GNULIB_VSCANF@ # if @REPLACE_STDIO_READ_FUNCS@ && @GNULIB_STDIO_H_NONBLOCKING@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef vscanf # define vscanf rpl_vscanf # endif _GL_FUNCDECL_RPL (vscanf, int, (const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_SCANF_SYSTEM (1, 0) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (vscanf, int, (const char *format, va_list args)); # else _GL_CXXALIAS_SYS (vscanf, int, (const char *format, va_list args)); # endif _GL_CXXALIASWARN (vscanf); #endif #if @GNULIB_VSNPRINTF@ # if @REPLACE_VSNPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vsnprintf rpl_vsnprintf # endif _GL_FUNCDECL_RPL (vsnprintf, int, (char *str, size_t size, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 0) _GL_ARG_NONNULL ((3))); _GL_CXXALIAS_RPL (vsnprintf, int, (char *str, size_t size, const char *format, va_list args)); # else # if !@HAVE_DECL_VSNPRINTF@ _GL_FUNCDECL_SYS (vsnprintf, int, (char *str, size_t size, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (3, 0) _GL_ARG_NONNULL ((3))); # endif _GL_CXXALIAS_SYS (vsnprintf, int, (char *str, size_t size, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vsnprintf); #elif defined GNULIB_POSIXCHECK # undef vsnprintf # if HAVE_RAW_DECL_VSNPRINTF _GL_WARN_ON_USE (vsnprintf, "vsnprintf is unportable - " "use gnulib module vsnprintf for portability"); # endif #endif #if @GNULIB_VSPRINTF_POSIX@ # if @REPLACE_VSPRINTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # define vsprintf rpl_vsprintf # endif _GL_FUNCDECL_RPL (vsprintf, int, (char *str, const char *format, va_list args) _GL_ATTRIBUTE_FORMAT_PRINTF (2, 0) _GL_ARG_NONNULL ((1, 2))); _GL_CXXALIAS_RPL (vsprintf, int, (char *str, const char *format, va_list args)); # else /* Need to cast, because on Solaris, the third parameter is __va_list args and GCC's fixincludes did not change this to __gnuc_va_list. */ _GL_CXXALIAS_SYS_CAST (vsprintf, int, (char *str, const char *format, va_list args)); # endif _GL_CXXALIASWARN (vsprintf); #elif defined GNULIB_POSIXCHECK # undef vsprintf /* Assume vsprintf is always declared. */ _GL_WARN_ON_USE (vsprintf, "vsprintf is not always POSIX compliant - " "use gnulib module vsprintf-posix for portable " "POSIX compliance"); #endif #endif /* _@GUARD_PREFIX@_STDIO_H */ #endif /* _@GUARD_PREFIX@_STDIO_H */ #endif gnuastro-0.5/bootstrapped/lib/stdint.in.h0000644000175000017500000005421713217200021015475 00000000000000/* Copyright (C) 2001-2002, 2004-2017 Free Software Foundation, Inc. Written by Paul Eggert, Bruno Haible, Sam Steingold, Peter Burwood. This file is part of gnulib. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* * ISO C 99 for platforms that lack it. * */ #ifndef _@GUARD_PREFIX@_STDINT_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* When including a system file that in turn includes , use the system , not our substitute. This avoids problems with (for example) VMS, whose includes . */ #define _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H /* On Android (Bionic libc), includes this file before having defined 'time_t'. Therefore in this case avoid including other system header files; just include the system's . Ideally we should test __BIONIC__ here, but it is only defined after has been included; hence test __ANDROID__ instead. */ #if defined __ANDROID__ && defined _GL_INCLUDING_SYS_TYPES_H # @INCLUDE_NEXT@ @NEXT_STDINT_H@ #else /* Get those types that are already defined in other system include files, so that we can "#define int8_t signed char" below without worrying about a later system include file containing a "typedef signed char int8_t;" that will get messed up by our macro. Our macros should all be consistent with the system versions, except for the "fast" types and macros, which we recommend against using in public interfaces due to compiler differences. */ #if @HAVE_STDINT_H@ # if defined __sgi && ! defined __c99 /* Bypass IRIX's if in C89 mode, since it merely annoys users with "This header file is to be used only for c99 mode compilations" diagnostics. */ # define __STDINT_H__ # endif /* Some pre-C++11 implementations need this. */ # ifdef __cplusplus # ifndef __STDC_CONSTANT_MACROS # define __STDC_CONSTANT_MACROS 1 # endif # ifndef __STDC_LIMIT_MACROS # define __STDC_LIMIT_MACROS 1 # endif # endif /* Other systems may have an incomplete or buggy . Include it before , since any "#include " in would reinclude us, skipping our contents because _@GUARD_PREFIX@_STDINT_H is defined. The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_STDINT_H@ #endif #if ! defined _@GUARD_PREFIX@_STDINT_H && ! defined _GL_JUST_INCLUDE_SYSTEM_STDINT_H #define _@GUARD_PREFIX@_STDINT_H /* Get SCHAR_MIN, SCHAR_MAX, UCHAR_MAX, INT_MIN, INT_MAX, LONG_MIN, LONG_MAX, ULONG_MAX, _GL_INTEGER_WIDTH. */ #include /* Override WINT_MIN and WINT_MAX if gnulib's or overrides wint_t. */ #if @GNULIB_OVERRIDES_WINT_T@ # undef WINT_MIN # undef WINT_MAX # define WINT_MIN 0x0U # define WINT_MAX 0xffffffffU #endif #if ! @HAVE_C99_STDINT_H@ /* defines some of the stdint.h types as well, on glibc, IRIX 6.5, and OpenBSD 3.8 (via ). AIX 5.2 isn't needed and causes troubles. Mac OS X 10.4.6 includes (which is us), but relies on the system definitions, so include after @NEXT_STDINT_H@. */ # if @HAVE_SYS_TYPES_H@ && ! defined _AIX # include # endif # if @HAVE_INTTYPES_H@ /* In OpenBSD 3.8, includes , which defines int{8,16,32,64}_t, uint{8,16,32,64}_t and __BIT_TYPES_DEFINED__. also defines intptr_t and uintptr_t. */ # include # elif @HAVE_SYS_INTTYPES_H@ /* Solaris 7 has the types except the *_fast*_t types, and the macros except for *_FAST*_*, INTPTR_MIN, PTRDIFF_MIN, PTRDIFF_MAX. */ # include # endif # if @HAVE_SYS_BITYPES_H@ && ! defined __BIT_TYPES_DEFINED__ /* Linux libc4 >= 4.6.7 and libc5 have a that defines int{8,16,32,64}_t and __BIT_TYPES_DEFINED__. In libc5 >= 5.2.2 it is included by . */ # include # endif # undef _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H /* Minimum and maximum values for an integer type under the usual assumption. Return an unspecified value if BITS == 0, adding a check to pacify picky compilers. */ /* These are separate macros, because if you try to merge these macros into a single one, HP-UX cc rejects the resulting expression in constant expressions. */ # define _STDINT_UNSIGNED_MIN(bits, zero) \ (zero) # define _STDINT_SIGNED_MIN(bits, zero) \ (~ _STDINT_MAX (1, bits, zero)) # define _STDINT_MAX(signed, bits, zero) \ (((((zero) + 1) << ((bits) ? (bits) - 1 - (signed) : 0)) - 1) * 2 + 1) #if !GNULIB_defined_stdint_types /* 7.18.1.1. Exact-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. */ # undef int8_t # undef uint8_t typedef signed char gl_int8_t; typedef unsigned char gl_uint8_t; # define int8_t gl_int8_t # define uint8_t gl_uint8_t # undef int16_t # undef uint16_t typedef short int gl_int16_t; typedef unsigned short int gl_uint16_t; # define int16_t gl_int16_t # define uint16_t gl_uint16_t # undef int32_t # undef uint32_t typedef int gl_int32_t; typedef unsigned int gl_uint32_t; # define int32_t gl_int32_t # define uint32_t gl_uint32_t /* If the system defines INT64_MAX, assume int64_t works. That way, if the underlying platform defines int64_t to be a 64-bit long long int, the code below won't mistakenly define it to be a 64-bit long int, which would mess up C++ name mangling. We must use #ifdef rather than #if, to avoid an error with HP-UX 10.20 cc. */ # ifdef INT64_MAX # define GL_INT64_T # else /* Do not undefine int64_t if gnulib is not being used with 64-bit types, since otherwise it breaks platforms like Tandem/NSK. */ # if LONG_MAX >> 31 >> 31 == 1 # undef int64_t typedef long int gl_int64_t; # define int64_t gl_int64_t # define GL_INT64_T # elif defined _MSC_VER # undef int64_t typedef __int64 gl_int64_t; # define int64_t gl_int64_t # define GL_INT64_T # elif @HAVE_LONG_LONG_INT@ # undef int64_t typedef long long int gl_int64_t; # define int64_t gl_int64_t # define GL_INT64_T # endif # endif # ifdef UINT64_MAX # define GL_UINT64_T # else # if ULONG_MAX >> 31 >> 31 >> 1 == 1 # undef uint64_t typedef unsigned long int gl_uint64_t; # define uint64_t gl_uint64_t # define GL_UINT64_T # elif defined _MSC_VER # undef uint64_t typedef unsigned __int64 gl_uint64_t; # define uint64_t gl_uint64_t # define GL_UINT64_T # elif @HAVE_UNSIGNED_LONG_LONG_INT@ # undef uint64_t typedef unsigned long long int gl_uint64_t; # define uint64_t gl_uint64_t # define GL_UINT64_T # endif # endif /* Avoid collision with Solaris 2.5.1 etc. */ # define _UINT8_T # define _UINT32_T # define _UINT64_T /* 7.18.1.2. Minimum-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the leastN_t types are the same as the corresponding N_t types. */ # undef int_least8_t # undef uint_least8_t # undef int_least16_t # undef uint_least16_t # undef int_least32_t # undef uint_least32_t # undef int_least64_t # undef uint_least64_t # define int_least8_t int8_t # define uint_least8_t uint8_t # define int_least16_t int16_t # define uint_least16_t uint16_t # define int_least32_t int32_t # define uint_least32_t uint32_t # ifdef GL_INT64_T # define int_least64_t int64_t # endif # ifdef GL_UINT64_T # define uint_least64_t uint64_t # endif /* 7.18.1.3. Fastest minimum-width integer types */ /* Note: Other substitutes may define these types differently. It is not recommended to use these types in public header files. */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the fastN_t types are taken from the same list of types. The following code normally uses types consistent with glibc, as that lessens the chance of incompatibility with older GNU hosts. */ # undef int_fast8_t # undef uint_fast8_t # undef int_fast16_t # undef uint_fast16_t # undef int_fast32_t # undef uint_fast32_t # undef int_fast64_t # undef uint_fast64_t typedef signed char gl_int_fast8_t; typedef unsigned char gl_uint_fast8_t; # ifdef __sun /* Define types compatible with SunOS 5.10, so that code compiled under earlier SunOS versions works with code compiled under SunOS 5.10. */ typedef int gl_int_fast32_t; typedef unsigned int gl_uint_fast32_t; # else typedef long int gl_int_fast32_t; typedef unsigned long int gl_uint_fast32_t; # endif typedef gl_int_fast32_t gl_int_fast16_t; typedef gl_uint_fast32_t gl_uint_fast16_t; # define int_fast8_t gl_int_fast8_t # define uint_fast8_t gl_uint_fast8_t # define int_fast16_t gl_int_fast16_t # define uint_fast16_t gl_uint_fast16_t # define int_fast32_t gl_int_fast32_t # define uint_fast32_t gl_uint_fast32_t # ifdef GL_INT64_T # define int_fast64_t int64_t # endif # ifdef GL_UINT64_T # define uint_fast64_t uint64_t # endif /* 7.18.1.4. Integer types capable of holding object pointers */ /* kLIBC's stdint.h defines _INTPTR_T_DECLARED and needs its own definitions of intptr_t and uintptr_t (which use int and unsigned) to avoid clashes with declarations of system functions like sbrk. */ # ifndef _INTPTR_T_DECLARED # undef intptr_t # undef uintptr_t typedef long int gl_intptr_t; typedef unsigned long int gl_uintptr_t; # define intptr_t gl_intptr_t # define uintptr_t gl_uintptr_t # endif /* 7.18.1.5. Greatest-width integer types */ /* Note: These types are compiler dependent. It may be unwise to use them in public header files. */ /* If the system defines INTMAX_MAX, assume that intmax_t works, and similarly for UINTMAX_MAX and uintmax_t. This avoids problems with assuming one type where another is used by the system. */ # ifndef INTMAX_MAX # undef INTMAX_C # undef intmax_t # if @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 typedef long long int gl_intmax_t; # define intmax_t gl_intmax_t # elif defined GL_INT64_T # define intmax_t int64_t # else typedef long int gl_intmax_t; # define intmax_t gl_intmax_t # endif # endif # ifndef UINTMAX_MAX # undef UINTMAX_C # undef uintmax_t # if @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 typedef unsigned long long int gl_uintmax_t; # define uintmax_t gl_uintmax_t # elif defined GL_UINT64_T # define uintmax_t uint64_t # else typedef unsigned long int gl_uintmax_t; # define uintmax_t gl_uintmax_t # endif # endif /* Verify that intmax_t and uintmax_t have the same size. Too much code breaks if this is not the case. If this check fails, the reason is likely to be found in the autoconf macros. */ typedef int _verify_intmax_size[sizeof (intmax_t) == sizeof (uintmax_t) ? 1 : -1]; # define GNULIB_defined_stdint_types 1 # endif /* !GNULIB_defined_stdint_types */ /* 7.18.2. Limits of specified-width integer types */ /* 7.18.2.1. Limits of exact-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. */ # undef INT8_MIN # undef INT8_MAX # undef UINT8_MAX # define INT8_MIN (~ INT8_MAX) # define INT8_MAX 127 # define UINT8_MAX 255 # undef INT16_MIN # undef INT16_MAX # undef UINT16_MAX # define INT16_MIN (~ INT16_MAX) # define INT16_MAX 32767 # define UINT16_MAX 65535 # undef INT32_MIN # undef INT32_MAX # undef UINT32_MAX # define INT32_MIN (~ INT32_MAX) # define INT32_MAX 2147483647 # define UINT32_MAX 4294967295U # if defined GL_INT64_T && ! defined INT64_MAX /* Prefer (- INTMAX_C (1) << 63) over (~ INT64_MAX) because SunPRO C 5.0 evaluates the latter incorrectly in preprocessor expressions. */ # define INT64_MIN (- INTMAX_C (1) << 63) # define INT64_MAX INTMAX_C (9223372036854775807) # endif # if defined GL_UINT64_T && ! defined UINT64_MAX # define UINT64_MAX UINTMAX_C (18446744073709551615) # endif /* 7.18.2.2. Limits of minimum-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the leastN_t types are the same as the corresponding N_t types. */ # undef INT_LEAST8_MIN # undef INT_LEAST8_MAX # undef UINT_LEAST8_MAX # define INT_LEAST8_MIN INT8_MIN # define INT_LEAST8_MAX INT8_MAX # define UINT_LEAST8_MAX UINT8_MAX # undef INT_LEAST16_MIN # undef INT_LEAST16_MAX # undef UINT_LEAST16_MAX # define INT_LEAST16_MIN INT16_MIN # define INT_LEAST16_MAX INT16_MAX # define UINT_LEAST16_MAX UINT16_MAX # undef INT_LEAST32_MIN # undef INT_LEAST32_MAX # undef UINT_LEAST32_MAX # define INT_LEAST32_MIN INT32_MIN # define INT_LEAST32_MAX INT32_MAX # define UINT_LEAST32_MAX UINT32_MAX # undef INT_LEAST64_MIN # undef INT_LEAST64_MAX # ifdef GL_INT64_T # define INT_LEAST64_MIN INT64_MIN # define INT_LEAST64_MAX INT64_MAX # endif # undef UINT_LEAST64_MAX # ifdef GL_UINT64_T # define UINT_LEAST64_MAX UINT64_MAX # endif /* 7.18.2.3. Limits of fastest minimum-width integer types */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits. Therefore the fastN_t types are taken from the same list of types. */ # undef INT_FAST8_MIN # undef INT_FAST8_MAX # undef UINT_FAST8_MAX # define INT_FAST8_MIN SCHAR_MIN # define INT_FAST8_MAX SCHAR_MAX # define UINT_FAST8_MAX UCHAR_MAX # undef INT_FAST16_MIN # undef INT_FAST16_MAX # undef UINT_FAST16_MAX # define INT_FAST16_MIN INT_FAST32_MIN # define INT_FAST16_MAX INT_FAST32_MAX # define UINT_FAST16_MAX UINT_FAST32_MAX # undef INT_FAST32_MIN # undef INT_FAST32_MAX # undef UINT_FAST32_MAX # ifdef __sun # define INT_FAST32_MIN INT_MIN # define INT_FAST32_MAX INT_MAX # define UINT_FAST32_MAX UINT_MAX # else # define INT_FAST32_MIN LONG_MIN # define INT_FAST32_MAX LONG_MAX # define UINT_FAST32_MAX ULONG_MAX # endif # undef INT_FAST64_MIN # undef INT_FAST64_MAX # ifdef GL_INT64_T # define INT_FAST64_MIN INT64_MIN # define INT_FAST64_MAX INT64_MAX # endif # undef UINT_FAST64_MAX # ifdef GL_UINT64_T # define UINT_FAST64_MAX UINT64_MAX # endif /* 7.18.2.4. Limits of integer types capable of holding object pointers */ # undef INTPTR_MIN # undef INTPTR_MAX # undef UINTPTR_MAX # define INTPTR_MIN LONG_MIN # define INTPTR_MAX LONG_MAX # define UINTPTR_MAX ULONG_MAX /* 7.18.2.5. Limits of greatest-width integer types */ # ifndef INTMAX_MAX # undef INTMAX_MIN # ifdef INT64_MAX # define INTMAX_MIN INT64_MIN # define INTMAX_MAX INT64_MAX # else # define INTMAX_MIN INT32_MIN # define INTMAX_MAX INT32_MAX # endif # endif # ifndef UINTMAX_MAX # ifdef UINT64_MAX # define UINTMAX_MAX UINT64_MAX # else # define UINTMAX_MAX UINT32_MAX # endif # endif /* 7.18.3. Limits of other integer types */ /* ptrdiff_t limits */ # undef PTRDIFF_MIN # undef PTRDIFF_MAX # if @APPLE_UNIVERSAL_BUILD@ # ifdef _LP64 # define PTRDIFF_MIN _STDINT_SIGNED_MIN (64, 0l) # define PTRDIFF_MAX _STDINT_MAX (1, 64, 0l) # else # define PTRDIFF_MIN _STDINT_SIGNED_MIN (32, 0) # define PTRDIFF_MAX _STDINT_MAX (1, 32, 0) # endif # else # define PTRDIFF_MIN \ _STDINT_SIGNED_MIN (@BITSIZEOF_PTRDIFF_T@, 0@PTRDIFF_T_SUFFIX@) # define PTRDIFF_MAX \ _STDINT_MAX (1, @BITSIZEOF_PTRDIFF_T@, 0@PTRDIFF_T_SUFFIX@) # endif /* sig_atomic_t limits */ # undef SIG_ATOMIC_MIN # undef SIG_ATOMIC_MAX # if @HAVE_SIGNED_SIG_ATOMIC_T@ # define SIG_ATOMIC_MIN \ _STDINT_SIGNED_MIN (@BITSIZEOF_SIG_ATOMIC_T@, 0@SIG_ATOMIC_T_SUFFIX@) # else # define SIG_ATOMIC_MIN \ _STDINT_UNSIGNED_MIN (@BITSIZEOF_SIG_ATOMIC_T@, 0@SIG_ATOMIC_T_SUFFIX@) # endif # define SIG_ATOMIC_MAX \ _STDINT_MAX (@HAVE_SIGNED_SIG_ATOMIC_T@, @BITSIZEOF_SIG_ATOMIC_T@, \ 0@SIG_ATOMIC_T_SUFFIX@) /* size_t limit */ # undef SIZE_MAX # if @APPLE_UNIVERSAL_BUILD@ # ifdef _LP64 # define SIZE_MAX _STDINT_MAX (0, 64, 0ul) # else # define SIZE_MAX _STDINT_MAX (0, 32, 0ul) # endif # else # define SIZE_MAX _STDINT_MAX (0, @BITSIZEOF_SIZE_T@, 0@SIZE_T_SUFFIX@) # endif /* wchar_t limits */ /* Get WCHAR_MIN, WCHAR_MAX. This include is not on the top, above, because on OSF/1 4.0 we have a sequence of nested includes -> -> -> , and the latter includes and assumes its types are already defined. */ # if @HAVE_WCHAR_H@ && ! (defined WCHAR_MIN && defined WCHAR_MAX) /* BSD/OS 4.0.1 has a bug: , and must be included before . */ # include # include # include # define _GL_JUST_INCLUDE_SYSTEM_WCHAR_H # include # undef _GL_JUST_INCLUDE_SYSTEM_WCHAR_H # endif # undef WCHAR_MIN # undef WCHAR_MAX # if @HAVE_SIGNED_WCHAR_T@ # define WCHAR_MIN \ _STDINT_SIGNED_MIN (@BITSIZEOF_WCHAR_T@, 0@WCHAR_T_SUFFIX@) # else # define WCHAR_MIN \ _STDINT_UNSIGNED_MIN (@BITSIZEOF_WCHAR_T@, 0@WCHAR_T_SUFFIX@) # endif # define WCHAR_MAX \ _STDINT_MAX (@HAVE_SIGNED_WCHAR_T@, @BITSIZEOF_WCHAR_T@, 0@WCHAR_T_SUFFIX@) /* wint_t limits */ # undef WINT_MIN # undef WINT_MAX # if @HAVE_SIGNED_WINT_T@ # define WINT_MIN \ _STDINT_SIGNED_MIN (@BITSIZEOF_WINT_T@, 0@WINT_T_SUFFIX@) # else # define WINT_MIN \ _STDINT_UNSIGNED_MIN (@BITSIZEOF_WINT_T@, 0@WINT_T_SUFFIX@) # endif # define WINT_MAX \ _STDINT_MAX (@HAVE_SIGNED_WINT_T@, @BITSIZEOF_WINT_T@, 0@WINT_T_SUFFIX@) /* 7.18.4. Macros for integer constants */ /* 7.18.4.1. Macros for minimum-width integer constants */ /* According to ISO C 99 Technical Corrigendum 1 */ /* Here we assume a standard architecture where the hardware integer types have 8, 16, 32, optionally 64 bits, and int is 32 bits. */ # undef INT8_C # undef UINT8_C # define INT8_C(x) x # define UINT8_C(x) x # undef INT16_C # undef UINT16_C # define INT16_C(x) x # define UINT16_C(x) x # undef INT32_C # undef UINT32_C # define INT32_C(x) x # define UINT32_C(x) x ## U # undef INT64_C # undef UINT64_C # if LONG_MAX >> 31 >> 31 == 1 # define INT64_C(x) x##L # elif defined _MSC_VER # define INT64_C(x) x##i64 # elif @HAVE_LONG_LONG_INT@ # define INT64_C(x) x##LL # endif # if ULONG_MAX >> 31 >> 31 >> 1 == 1 # define UINT64_C(x) x##UL # elif defined _MSC_VER # define UINT64_C(x) x##ui64 # elif @HAVE_UNSIGNED_LONG_LONG_INT@ # define UINT64_C(x) x##ULL # endif /* 7.18.4.2. Macros for greatest-width integer constants */ # ifndef INTMAX_C # if @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 # define INTMAX_C(x) x##LL # elif defined GL_INT64_T # define INTMAX_C(x) INT64_C(x) # else # define INTMAX_C(x) x##L # endif # endif # ifndef UINTMAX_C # if @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 # define UINTMAX_C(x) x##ULL # elif defined GL_UINT64_T # define UINTMAX_C(x) UINT64_C(x) # else # define UINTMAX_C(x) x##UL # endif # endif #endif /* !@HAVE_C99_STDINT_H@ */ /* Macros specified by ISO/IEC TS 18661-1:2014. */ #if (!defined UINTMAX_WIDTH \ && (defined _GNU_SOURCE || defined __STDC_WANT_IEC_60559_BFP_EXT__)) # ifdef INT8_MAX # define INT8_WIDTH _GL_INTEGER_WIDTH (INT8_MIN, INT8_MAX) # endif # ifdef UINT8_MAX # define UINT8_WIDTH _GL_INTEGER_WIDTH (0, UINT8_MAX) # endif # ifdef INT16_MAX # define INT16_WIDTH _GL_INTEGER_WIDTH (INT16_MIN, INT16_MAX) # endif # ifdef UINT16_MAX # define UINT16_WIDTH _GL_INTEGER_WIDTH (0, UINT16_MAX) # endif # ifdef INT32_MAX # define INT32_WIDTH _GL_INTEGER_WIDTH (INT32_MIN, INT32_MAX) # endif # ifdef UINT32_MAX # define UINT32_WIDTH _GL_INTEGER_WIDTH (0, UINT32_MAX) # endif # ifdef INT64_MAX # define INT64_WIDTH _GL_INTEGER_WIDTH (INT64_MIN, INT64_MAX) # endif # ifdef UINT64_MAX # define UINT64_WIDTH _GL_INTEGER_WIDTH (0, UINT64_MAX) # endif # define INT_LEAST8_WIDTH _GL_INTEGER_WIDTH (INT_LEAST8_MIN, INT_LEAST8_MAX) # define UINT_LEAST8_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST8_MAX) # define INT_LEAST16_WIDTH _GL_INTEGER_WIDTH (INT_LEAST16_MIN, INT_LEAST16_MAX) # define UINT_LEAST16_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST16_MAX) # define INT_LEAST32_WIDTH _GL_INTEGER_WIDTH (INT_LEAST32_MIN, INT_LEAST32_MAX) # define UINT_LEAST32_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST32_MAX) # define INT_LEAST64_WIDTH _GL_INTEGER_WIDTH (INT_LEAST64_MIN, INT_LEAST64_MAX) # define UINT_LEAST64_WIDTH _GL_INTEGER_WIDTH (0, UINT_LEAST64_MAX) # define INT_FAST8_WIDTH _GL_INTEGER_WIDTH (INT_FAST8_MIN, INT_FAST8_MAX) # define UINT_FAST8_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST8_MAX) # define INT_FAST16_WIDTH _GL_INTEGER_WIDTH (INT_FAST16_MIN, INT_FAST16_MAX) # define UINT_FAST16_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST16_MAX) # define INT_FAST32_WIDTH _GL_INTEGER_WIDTH (INT_FAST32_MIN, INT_FAST32_MAX) # define UINT_FAST32_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST32_MAX) # define INT_FAST64_WIDTH _GL_INTEGER_WIDTH (INT_FAST64_MIN, INT_FAST64_MAX) # define UINT_FAST64_WIDTH _GL_INTEGER_WIDTH (0, UINT_FAST64_MAX) # define INTPTR_WIDTH _GL_INTEGER_WIDTH (INTPTR_MIN, INTPTR_MAX) # define UINTPTR_WIDTH _GL_INTEGER_WIDTH (0, UINTPTR_MAX) # define INTMAX_WIDTH _GL_INTEGER_WIDTH (INTMAX_MIN, INTMAX_MAX) # define UINTMAX_WIDTH _GL_INTEGER_WIDTH (0, UINTMAX_MAX) # define PTRDIFF_WIDTH _GL_INTEGER_WIDTH (PTRDIFF_MIN, PTRDIFF_MAX) # define SIZE_WIDTH _GL_INTEGER_WIDTH (0, SIZE_MAX) # define WCHAR_WIDTH _GL_INTEGER_WIDTH (WCHAR_MIN, WCHAR_MAX) # ifdef WINT_MAX # define WINT_WIDTH _GL_INTEGER_WIDTH (WINT_MIN, WINT_MAX) # endif # ifdef SIG_ATOMIC_MAX # define SIG_ATOMIC_WIDTH _GL_INTEGER_WIDTH (SIG_ATOMIC_MIN, SIG_ATOMIC_MAX) # endif #endif /* !WINT_WIDTH && (_GNU_SOURCE || __STDC_WANT_IEC_60559_BFP_EXT__) */ #endif /* _@GUARD_PREFIX@_STDINT_H */ #endif /* !(defined __ANDROID__ && ...) */ #endif /* !defined _@GUARD_PREFIX@_STDINT_H && !defined _GL_JUST_INCLUDE_SYSTEM_STDINT_H */ gnuastro-0.5/bootstrapped/lib/stddef.in.h0000644000175000017500000000746313217200021015442 00000000000000/* A substitute for POSIX 2008 , for platforms that have issues. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Eric Blake. */ /* * POSIX 2008 for platforms that have issues. * */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #if defined __need_wchar_t || defined __need_size_t \ || defined __need_ptrdiff_t || defined __need_NULL \ || defined __need_wint_t /* Special invocation convention inside gcc header files. In particular, gcc provides a version of that blindly redefines NULL even when __need_wint_t was defined, even though wint_t is not normally provided by . Hence, we must remember if special invocation has ever been used to obtain wint_t, in which case we need to clean up NULL yet again. */ # if !(defined _@GUARD_PREFIX@_STDDEF_H && defined _GL_STDDEF_WINT_T) # ifdef __need_wint_t # define _GL_STDDEF_WINT_T # endif # @INCLUDE_NEXT@ @NEXT_STDDEF_H@ # endif #else /* Normal invocation convention. */ # ifndef _@GUARD_PREFIX@_STDDEF_H /* The include_next requires a split double-inclusion guard. */ # @INCLUDE_NEXT@ @NEXT_STDDEF_H@ /* On NetBSD 5.0, the definition of NULL lacks proper parentheses. */ # if (@REPLACE_NULL@ \ && (!defined _@GUARD_PREFIX@_STDDEF_H || defined _GL_STDDEF_WINT_T)) # undef NULL # ifdef __cplusplus /* ISO C++ says that the macro NULL must expand to an integer constant expression, hence '((void *) 0)' is not allowed in C++. */ # if __GNUG__ >= 3 /* GNU C++ has a __null macro that behaves like an integer ('int' or 'long') but has the same size as a pointer. Use that, to avoid warnings. */ # define NULL __null # else # define NULL 0L # endif # else # define NULL ((void *) 0) # endif # endif # ifndef _@GUARD_PREFIX@_STDDEF_H # define _@GUARD_PREFIX@_STDDEF_H /* Some platforms lack wchar_t. */ #if !@HAVE_WCHAR_T@ # define wchar_t int #endif /* Some platforms lack max_align_t. The check for _GCC_MAX_ALIGN_T is a hack in case the configure-time test was done with g++ even though we are currently compiling with gcc. */ #if ! (@HAVE_MAX_ALIGN_T@ || defined _GCC_MAX_ALIGN_T) # if !GNULIB_defined_max_align_t /* On the x86, the maximum storage alignment of double, long, etc. is 4, but GCC's C11 ABI for x86 says that max_align_t has an alignment of 8, and the C11 standard allows this. Work around this problem by using __alignof__ (which returns 8 for double) rather than _Alignof (which returns 4), and align each union member accordingly. */ # ifdef __GNUC__ # define _GL_STDDEF_ALIGNAS(type) \ __attribute__ ((__aligned__ (__alignof__ (type)))) # else # define _GL_STDDEF_ALIGNAS(type) /* */ # endif typedef union { char *__p _GL_STDDEF_ALIGNAS (char *); double __d _GL_STDDEF_ALIGNAS (double); long double __ld _GL_STDDEF_ALIGNAS (long double); long int __i _GL_STDDEF_ALIGNAS (long int); } rpl_max_align_t; # define max_align_t rpl_max_align_t # define GNULIB_defined_max_align_t 1 # endif #endif # endif /* _@GUARD_PREFIX@_STDDEF_H */ # endif /* _@GUARD_PREFIX@_STDDEF_H */ #endif /* __need_XXX */ gnuastro-0.5/bootstrapped/lib/stdbool.in.h0000644000175000017500000001175013217200021015631 00000000000000/* Copyright (C) 2001-2003, 2006-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2001. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _GL_STDBOOL_H #define _GL_STDBOOL_H /* ISO C 99 for platforms that lack it. */ /* Usage suggestions: Programs that use should be aware of some limitations and standards compliance issues. Standards compliance: - must be #included before 'bool', 'false', 'true' can be used. - You cannot assume that sizeof (bool) == 1. - Programs should not undefine the macros bool, true, and false, as C99 lists that as an "obsolescent feature". Limitations of this substitute, when used in a C89 environment: - must be #included before the '_Bool' type can be used. - You cannot assume that _Bool is a typedef; it might be a macro. - Bit-fields of type 'bool' are not supported. Portable code should use 'unsigned int foo : 1;' rather than 'bool foo : 1;'. - In C99, casts and automatic conversions to '_Bool' or 'bool' are performed in such a way that every nonzero value gets converted to 'true', and zero gets converted to 'false'. This doesn't work with this substitute. With this substitute, only the values 0 and 1 give the expected result when converted to _Bool' or 'bool'. - C99 allows the use of (_Bool)0.0 in constant expressions, but this substitute cannot always provide this property. Also, it is suggested that programs use 'bool' rather than '_Bool'; this isn't required, but 'bool' is more common. */ /* 7.16. Boolean type and values */ /* BeOS already #defines false 0, true 1. We use the same definitions below, but temporarily we have to #undef them. */ #if defined __BEOS__ && !defined __HAIKU__ # include /* defines bool but not _Bool */ # undef false # undef true #endif #ifdef __cplusplus # define _Bool bool # define bool bool #else # if defined __BEOS__ && !defined __HAIKU__ /* A compiler known to have 'bool'. */ /* If the compiler already has both 'bool' and '_Bool', we can assume they are the same types. */ # if !@HAVE__BOOL@ typedef bool _Bool; # endif # else # if !defined __GNUC__ /* If @HAVE__BOOL@: Some HP-UX cc and AIX IBM C compiler versions have compiler bugs when the built-in _Bool type is used. See https://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html https://lists.gnu.org/r/bug-coreutils/2005-11/msg00161.html https://lists.gnu.org/r/bug-coreutils/2005-10/msg00086.html Similar bugs are likely with other compilers as well; this file wouldn't be used if was working. So we override the _Bool type. If !@HAVE__BOOL@: Need to define _Bool ourselves. As 'signed char' or as an enum type? Use of a typedef, with SunPRO C, leads to a stupid "warning: _Bool is a keyword in ISO C99". Use of an enum type, with IRIX cc, leads to a stupid "warning(1185): enumerated type mixed with another type". Even the existence of an enum type, without a typedef, "Invalid enumerator. (badenum)" with HP-UX cc on Tru64. The only benefit of the enum, debuggability, is not important with these compilers. So use 'signed char' and no enum. */ # define _Bool signed char # else /* With this compiler, trust the _Bool type if the compiler has it. */ # if !@HAVE__BOOL@ /* For the sake of symbolic names in gdb, define true and false as enum constants, not only as macros. It is tempting to write typedef enum { false = 0, true = 1 } _Bool; so that gdb prints values of type 'bool' symbolically. But then values of type '_Bool' might promote to 'int' or 'unsigned int' (see ISO C 99 6.7.2.2.(4)); however, '_Bool' must promote to 'int' (see ISO C 99 6.3.1.1.(2)). So add a negative value to the enum; this ensures that '_Bool' promotes to 'int'. */ typedef enum { _Bool_must_promote_to_int = -1, false = 0, true = 1 } _Bool; # endif # endif # endif # define bool _Bool #endif /* The other macros must be usable in preprocessor directives. */ #ifdef __cplusplus # define false false # define true true #else # define false 0 # define true 1 #endif #define __bool_true_false_are_defined 1 #endif /* _GL_STDBOOL_H */ gnuastro-0.5/bootstrapped/lib/stdalign.in.h0000644000175000017500000001117013217200021015764 00000000000000/* A substitute for ISO C11 . Copyright 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Paul Eggert and Bruno Haible. */ #ifndef _GL_STDALIGN_H #define _GL_STDALIGN_H /* ISO C11 for platforms that lack it. References: ISO C11 (latest free draft ) sections 6.5.3.4, 6.7.5, 7.15. C++11 (latest free draft ) section 18.10. */ /* alignof (TYPE), also known as _Alignof (TYPE), yields the alignment requirement of a structure member (i.e., slot or field) that is of type TYPE, as an integer constant expression. This differs from GCC's __alignof__ operator, which can yield a better-performing alignment for an object of that type. For example, on x86 with GCC, __alignof__ (double) and __alignof__ (long long) are 8, whereas alignof (double) and alignof (long long) are 4 unless the option '-malign-double' is used. The result cannot be used as a value for an 'enum' constant, if you want to be portable to HP-UX 10.20 cc and AIX 3.2.5 xlc. Include for offsetof. */ #include /* FreeBSD 9.1 , included by and lots of other standard headers, defines conflicting implementations of _Alignas and _Alignof that are no better than ours; override them. */ #undef _Alignas #undef _Alignof /* GCC releases before GCC 4.9 had a bug in _Alignof. See GCC bug 52023 . */ #if (!defined __STDC_VERSION__ || __STDC_VERSION__ < 201112 \ || (defined __GNUC__ && __GNUC__ < 4 + (__GNUC_MINOR__ < 9))) # ifdef __cplusplus # if 201103 <= __cplusplus # define _Alignof(type) alignof (type) # else template struct __alignof_helper { char __a; __t __b; }; # define _Alignof(type) offsetof (__alignof_helper, __b) # endif # else # define _Alignof(type) offsetof (struct { char __a; type __b; }, __b) # endif #endif #if ! (defined __cplusplus && 201103 <= __cplusplus) # define alignof _Alignof #endif #define __alignof_is_defined 1 /* alignas (A), also known as _Alignas (A), aligns a variable or type to the alignment A, where A is an integer constant expression. For example: int alignas (8) foo; struct s { int a; int alignas (8) bar; }; aligns the address of FOO and the offset of BAR to be multiples of 8. A should be a power of two that is at least the type's alignment and at most the implementation's alignment limit. This limit is 2**28 on typical GNUish hosts, and 2**13 on MSVC. To be portable to MSVC through at least version 10.0, A should be an integer constant, as MSVC does not support expressions such as 1 << 3. To be portable to Sun C 5.11, do not align auto variables to anything stricter than their default alignment. The following C11 requirements are not supported here: - If A is zero, alignas has no effect. - alignas can be used multiple times; the strictest one wins. - alignas (TYPE) is equivalent to alignas (alignof (TYPE)). */ #if !defined __STDC_VERSION__ || __STDC_VERSION__ < 201112 # if defined __cplusplus && 201103 <= __cplusplus # define _Alignas(a) alignas (a) # elif ((defined __APPLE__ && defined __MACH__ \ ? 4 < __GNUC__ + (1 <= __GNUC_MINOR__) \ : __GNUC__) \ || (__ia64 && (61200 <= __HP_cc || 61200 <= __HP_aCC)) \ || __ICC || 0x590 <= __SUNPRO_C || 0x0600 <= __xlC__) # define _Alignas(a) __attribute__ ((__aligned__ (a))) # elif 1300 <= _MSC_VER # define _Alignas(a) __declspec (align (a)) # endif #endif #if ((defined _Alignas && ! (defined __cplusplus && 201103 <= __cplusplus)) \ || (defined __STDC_VERSION__ && 201112 <= __STDC_VERSION__)) # define alignas _Alignas #endif #if defined alignas || (defined __cplusplus && 201103 <= __cplusplus) # define __alignas_is_defined 1 #endif #endif /* _GL_STDALIGN_H */ gnuastro-0.5/bootstrapped/lib/warn-on-use.h0000644000175000017500000001201013217200022015720 00000000000000/* A C macro for emitting warnings if a function is used. Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* _GL_WARN_ON_USE (function, "literal string") issues a declaration for FUNCTION which will then trigger a compiler warning containing the text of "literal string" anywhere that function is called, if supported by the compiler. If the compiler does not support this feature, the macro expands to an unused extern declaration. This macro is useful for marking a function as a potential portability trap, with the intent that "literal string" include instructions on the replacement function that should be used instead. However, one of the reasons that a function is a portability trap is if it has the wrong signature. Declaring FUNCTION with a different signature in C is a compilation error, so this macro must use the same type as any existing declaration so that programs that avoid the problematic FUNCTION do not fail to compile merely because they included a header that poisoned the function. But this implies that _GL_WARN_ON_USE is only safe to use if FUNCTION is known to already have a declaration. Use of this macro implies that there must not be any other macro hiding the declaration of FUNCTION; but undefining FUNCTION first is part of the poisoning process anyway (although for symbols that are provided only via a macro, the result is a compilation error rather than a warning containing "literal string"). Also note that in C++, it is only safe to use if FUNCTION has no overloads. For an example, it is possible to poison 'getline' by: - adding a call to gl_WARN_ON_USE_PREPARE([[#include ]], [getline]) in configure.ac, which potentially defines HAVE_RAW_DECL_GETLINE - adding this code to a header that wraps the system : #undef getline #if HAVE_RAW_DECL_GETLINE _GL_WARN_ON_USE (getline, "getline is required by POSIX 2008, but" "not universally present; use the gnulib module getline"); #endif It is not possible to directly poison global variables. But it is possible to write a wrapper accessor function, and poison that (less common usage, like &environ, will cause a compilation error rather than issue the nice warning, but the end result of informing the developer about their portability problem is still achieved): #if HAVE_RAW_DECL_ENVIRON static char ***rpl_environ (void) { return &environ; } _GL_WARN_ON_USE (rpl_environ, "environ is not always properly declared"); # undef environ # define environ (*rpl_environ ()) #endif */ #ifndef _GL_WARN_ON_USE # if 4 < __GNUC__ || (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) /* A compiler attribute is available in gcc versions 4.3.0 and later. */ # define _GL_WARN_ON_USE(function, message) \ extern __typeof__ (function) function __attribute__ ((__warning__ (message))) # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING /* Verify the existence of the function. */ # define _GL_WARN_ON_USE(function, message) \ extern __typeof__ (function) function # else /* Unsupported. */ # define _GL_WARN_ON_USE(function, message) \ _GL_WARN_EXTERN_C int _gl_warn_on_use # endif #endif /* _GL_WARN_ON_USE_CXX (function, rettype, parameters_and_attributes, "string") is like _GL_WARN_ON_USE (function, "string"), except that the function is declared with the given prototype, consisting of return type, parameters, and attributes. This variant is useful for overloaded functions in C++. _GL_WARN_ON_USE does not work in this case. */ #ifndef _GL_WARN_ON_USE_CXX # if 4 < __GNUC__ || (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ extern rettype function parameters_and_attributes \ __attribute__ ((__warning__ (msg))) # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING /* Verify the existence of the function. */ # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ extern rettype function parameters_and_attributes # else /* Unsupported. */ # define _GL_WARN_ON_USE_CXX(function,rettype,parameters_and_attributes,msg) \ _GL_WARN_EXTERN_C int _gl_warn_on_use # endif #endif /* _GL_WARN_EXTERN_C declaration; performs the declaration with C linkage. */ #ifndef _GL_WARN_EXTERN_C # if defined __cplusplus # define _GL_WARN_EXTERN_C extern "C" # else # define _GL_WARN_EXTERN_C extern # endif #endif gnuastro-0.5/bootstrapped/lib/c++defs.h0000644000175000017500000003413013217200020014764 00000000000000/* C++ compatible function declaration macros. Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_CXXDEFS_H #define _GL_CXXDEFS_H /* Begin/end the GNULIB_NAMESPACE namespace. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_BEGIN_NAMESPACE namespace GNULIB_NAMESPACE { # define _GL_END_NAMESPACE } #else # define _GL_BEGIN_NAMESPACE # define _GL_END_NAMESPACE #endif /* The three most frequent use cases of these macros are: * For providing a substitute for a function that is missing on some platforms, but is declared and works fine on the platforms on which it exists: #if @GNULIB_FOO@ # if !@HAVE_FOO@ _GL_FUNCDECL_SYS (foo, ...); # endif _GL_CXXALIAS_SYS (foo, ...); _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif * For providing a replacement for a function that exists on all platforms, but is broken/insufficient and needs to be replaced on some platforms: #if @GNULIB_FOO@ # if @REPLACE_FOO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef foo # define foo rpl_foo # endif _GL_FUNCDECL_RPL (foo, ...); _GL_CXXALIAS_RPL (foo, ...); # else _GL_CXXALIAS_SYS (foo, ...); # endif _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif * For providing a replacement for a function that exists on some platforms but is broken/insufficient and needs to be replaced on some of them and is additionally either missing or undeclared on some other platforms: #if @GNULIB_FOO@ # if @REPLACE_FOO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef foo # define foo rpl_foo # endif _GL_FUNCDECL_RPL (foo, ...); _GL_CXXALIAS_RPL (foo, ...); # else # if !@HAVE_FOO@ or if !@HAVE_DECL_FOO@ _GL_FUNCDECL_SYS (foo, ...); # endif _GL_CXXALIAS_SYS (foo, ...); # endif _GL_CXXALIASWARN (foo); #elif defined GNULIB_POSIXCHECK ... #endif */ /* _GL_EXTERN_C declaration; performs the declaration with C linkage. */ #if defined __cplusplus # define _GL_EXTERN_C extern "C" #else # define _GL_EXTERN_C extern #endif /* _GL_FUNCDECL_RPL (func, rettype, parameters_and_attributes); declares a replacement function, named rpl_func, with the given prototype, consisting of return type, parameters, and attributes. Example: _GL_FUNCDECL_RPL (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); */ #define _GL_FUNCDECL_RPL(func,rettype,parameters_and_attributes) \ _GL_FUNCDECL_RPL_1 (rpl_##func, rettype, parameters_and_attributes) #define _GL_FUNCDECL_RPL_1(rpl_func,rettype,parameters_and_attributes) \ _GL_EXTERN_C rettype rpl_func parameters_and_attributes /* _GL_FUNCDECL_SYS (func, rettype, parameters_and_attributes); declares the system function, named func, with the given prototype, consisting of return type, parameters, and attributes. Example: _GL_FUNCDECL_SYS (open, int, (const char *filename, int flags, ...) _GL_ARG_NONNULL ((1))); */ #define _GL_FUNCDECL_SYS(func,rettype,parameters_and_attributes) \ _GL_EXTERN_C rettype func parameters_and_attributes /* _GL_CXXALIAS_RPL (func, rettype, parameters); declares a C++ alias called GNULIB_NAMESPACE::func that redirects to rpl_func, if GNULIB_NAMESPACE is defined. Example: _GL_CXXALIAS_RPL (open, int, (const char *filename, int flags, ...)); Wrapping rpl_func in an object with an inline conversion operator avoids a reference to rpl_func unless GNULIB_NAMESPACE::func is actually used in the program. */ #define _GL_CXXALIAS_RPL(func,rettype,parameters) \ _GL_CXXALIAS_RPL_1 (func, rpl_##func, rettype, parameters) #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_RPL_1(func,rpl_func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return ::rpl_func; \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_RPL_1(func,rpl_func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_RPL_CAST_1 (func, rpl_func, rettype, parameters); is like _GL_CXXALIAS_RPL_1 (func, rpl_func, rettype, parameters); except that the C function rpl_func may have a slightly different declaration. A cast is used to silence the "invalid conversion" error that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_RPL_CAST_1(func,rpl_func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return reinterpret_cast(::rpl_func); \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_RPL_CAST_1(func,rpl_func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS (func, rettype, parameters); declares a C++ alias called GNULIB_NAMESPACE::func that redirects to the system provided function func, if GNULIB_NAMESPACE is defined. Example: _GL_CXXALIAS_SYS (open, int, (const char *filename, int flags, ...)); Wrapping func in an object with an inline conversion operator avoids a reference to func unless GNULIB_NAMESPACE::func is actually used in the program. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_SYS(func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return ::func; \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS(func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS_CAST (func, rettype, parameters); is like _GL_CXXALIAS_SYS (func, rettype, parameters); except that the C function func may have a slightly different declaration. A cast is used to silence the "invalid conversion" error that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIAS_SYS_CAST(func,rettype,parameters) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return reinterpret_cast(::func); \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS_CAST(func,rettype,parameters) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIAS_SYS_CAST2 (func, rettype, parameters, rettype2, parameters2); is like _GL_CXXALIAS_SYS (func, rettype, parameters); except that the C function is picked among a set of overloaded functions, namely the one with rettype2 and parameters2. Two consecutive casts are used to silence the "cannot find a match" and "invalid conversion" errors that would otherwise occur. */ #if defined __cplusplus && defined GNULIB_NAMESPACE /* The outer cast must be a reinterpret_cast. The inner cast: When the function is defined as a set of overloaded functions, it works as a static_cast<>, choosing the designated variant. When the function is defined as a single variant, it works as a reinterpret_cast<>. The parenthesized cast syntax works both ways. */ # define _GL_CXXALIAS_SYS_CAST2(func,rettype,parameters,rettype2,parameters2) \ namespace GNULIB_NAMESPACE \ { \ static const struct _gl_ ## func ## _wrapper \ { \ typedef rettype (*type) parameters; \ \ inline operator type () const \ { \ return reinterpret_cast((rettype2 (*) parameters2)(::func)); \ } \ } func = {}; \ } \ _GL_EXTERN_C int _gl_cxxalias_dummy #else # define _GL_CXXALIAS_SYS_CAST2(func,rettype,parameters,rettype2,parameters2) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIASWARN (func); causes a warning to be emitted when ::func is used but not when GNULIB_NAMESPACE::func is used. func must be defined without overloaded variants. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIASWARN(func) \ _GL_CXXALIASWARN_1 (func, GNULIB_NAMESPACE) # define _GL_CXXALIASWARN_1(func,namespace) \ _GL_CXXALIASWARN_2 (func, namespace) /* To work around GCC bug , we enable the warning only when not optimizing. */ # if !__OPTIMIZE__ # define _GL_CXXALIASWARN_2(func,namespace) \ _GL_WARN_ON_USE (func, \ "The symbol ::" #func " refers to the system function. " \ "Use " #namespace "::" #func " instead.") # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING # define _GL_CXXALIASWARN_2(func,namespace) \ extern __typeof__ (func) func # else # define _GL_CXXALIASWARN_2(func,namespace) \ _GL_EXTERN_C int _gl_cxxalias_dummy # endif #else # define _GL_CXXALIASWARN(func) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif /* _GL_CXXALIASWARN1 (func, rettype, parameters_and_attributes); causes a warning to be emitted when the given overloaded variant of ::func is used but not when GNULIB_NAMESPACE::func is used. */ #if defined __cplusplus && defined GNULIB_NAMESPACE # define _GL_CXXALIASWARN1(func,rettype,parameters_and_attributes) \ _GL_CXXALIASWARN1_1 (func, rettype, parameters_and_attributes, \ GNULIB_NAMESPACE) # define _GL_CXXALIASWARN1_1(func,rettype,parameters_and_attributes,namespace) \ _GL_CXXALIASWARN1_2 (func, rettype, parameters_and_attributes, namespace) /* To work around GCC bug , we enable the warning only when not optimizing. */ # if !__OPTIMIZE__ # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ _GL_WARN_ON_USE_CXX (func, rettype, parameters_and_attributes, \ "The symbol ::" #func " refers to the system function. " \ "Use " #namespace "::" #func " instead.") # elif __GNUC__ >= 3 && GNULIB_STRICT_CHECKING # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ extern __typeof__ (func) func # else # define _GL_CXXALIASWARN1_2(func,rettype,parameters_and_attributes,namespace) \ _GL_EXTERN_C int _gl_cxxalias_dummy # endif #else # define _GL_CXXALIASWARN1(func,rettype,parameters_and_attributes) \ _GL_EXTERN_C int _gl_cxxalias_dummy #endif #endif /* _GL_CXXDEFS_H */ gnuastro-0.5/bootstrapped/lib/arg-nonnull.h0000644000175000017500000000230113217200020016001 00000000000000/* A C macro for declaring that specific arguments must not be NULL. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* _GL_ARG_NONNULL((n,...,m)) tells the compiler and static analyzer tools that the values passed as arguments n, ..., m must be non-NULL pointers. n = 1 stands for the first argument, n = 2 for the second argument etc. */ #ifndef _GL_ARG_NONNULL # if (__GNUC__ == 3 && __GNUC_MINOR__ >= 3) || __GNUC__ > 3 # define _GL_ARG_NONNULL(params) __attribute__ ((__nonnull__ params)) # else # define _GL_ARG_NONNULL(params) # endif #endif gnuastro-0.5/bootstrapped/lib/_Noreturn.h0000644000175000017500000000046213217200020015526 00000000000000#if !defined _Noreturn && __STDC_VERSION__ < 201112 # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif gnuastro-0.5/bootstrapped/lib/regex_internal.h0000644000175000017500000006167513217200021016577 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _REGEX_INTERNAL_H #define _REGEX_INTERNAL_H 1 #include #include #include #include #include #include #include #include #include #include #include #include "intprops.h" #ifdef _LIBC # include # define lock_define(name) __libc_lock_define (, name) # define lock_init(lock) (__libc_lock_init (lock), 0) # define lock_fini(lock) 0 # define lock_lock(lock) __libc_lock_lock (lock) # define lock_unlock(lock) __libc_lock_unlock (lock) #elif defined GNULIB_LOCK && !defined USE_UNLOCKED_IO # include "glthread/lock.h" /* Use gl_lock_define if empty macro arguments are known to work. Otherwise, fall back on less-portable substitutes. */ # if ((defined __GNUC__ && !defined __STRICT_ANSI__) \ || (defined __STDC_VERSION__ && 199901L <= __STDC_VERSION__)) # define lock_define(name) gl_lock_define (, name) # elif USE_POSIX_THREADS # define lock_define(name) pthread_mutex_t name; # elif USE_PTH_THREADS # define lock_define(name) pth_mutex_t name; # elif USE_SOLARIS_THREADS # define lock_define(name) mutex_t name; # elif USE_WINDOWS_THREADS # define lock_define(name) gl_lock_t name; # else # define lock_define(name) # endif # define lock_init(lock) glthread_lock_init (&(lock)) # define lock_fini(lock) glthread_lock_destroy (&(lock)) # define lock_lock(lock) glthread_lock_lock (&(lock)) # define lock_unlock(lock) glthread_lock_unlock (&(lock)) #elif defined GNULIB_PTHREAD && !defined USE_UNLOCKED_IO # include # define lock_define(name) pthread_mutex_t name; # define lock_init(lock) pthread_mutex_init (&(lock), 0) # define lock_fini(lock) pthread_mutex_destroy (&(lock)) # define lock_lock(lock) pthread_mutex_lock (&(lock)) # define lock_unlock(lock) pthread_mutex_unlock (&(lock)) #else # define lock_define(name) # define lock_init(lock) 0 # define lock_fini(lock) ((void) 0) /* The 'dfa' avoids an "unused variable 'dfa'" warning from GCC. */ # define lock_lock(lock) ((void) dfa) # define lock_unlock(lock) ((void) 0) #endif /* In case that the system doesn't have isblank(). */ #if !defined _LIBC && ! (defined isblank || (HAVE_ISBLANK && HAVE_DECL_ISBLANK)) # define isblank(ch) ((ch) == ' ' || (ch) == '\t') #endif #ifdef _LIBC # ifndef _RE_DEFINE_LOCALE_FUNCTIONS # define _RE_DEFINE_LOCALE_FUNCTIONS 1 # include # include # endif #endif /* This is for other GNU distributions with internationalized messages. */ #if (HAVE_LIBINTL_H && ENABLE_NLS) || defined _LIBC # include # ifdef _LIBC # undef gettext # define gettext(msgid) \ __dcgettext (_libc_intl_domainname, msgid, LC_MESSAGES) # endif #else # undef gettext # define gettext(msgid) (msgid) #endif #ifndef gettext_noop /* This define is so xgettext can find the internationalizable strings. */ # define gettext_noop(String) String #endif #if (defined MB_CUR_MAX && HAVE_WCTYPE_H && HAVE_ISWCTYPE) || _LIBC # define RE_ENABLE_I18N #endif #define BE(expr, val) __builtin_expect (expr, val) /* Number of ASCII characters. */ #define ASCII_CHARS 0x80 /* Number of single byte characters. */ #define SBC_MAX (UCHAR_MAX + 1) #define COLL_ELEM_LEN_MAX 8 /* The character which represents newline. */ #define NEWLINE_CHAR '\n' #define WIDE_NEWLINE_CHAR L'\n' /* Rename to standard API for using out of glibc. */ #ifndef _LIBC # undef __wctype # undef __iswctype # define __wctype wctype # define __iswalnum iswalnum # define __iswctype iswctype # define __towlower towlower # define __towupper towupper # define __btowc btowc # define __mbrtowc mbrtowc # define __wcrtomb wcrtomb # define __regfree regfree # define attribute_hidden #endif /* not _LIBC */ #if __GNUC__ < 3 + (__GNUC_MINOR__ < 1) # define __attribute__(arg) #endif #ifndef SSIZE_MAX # define SSIZE_MAX ((ssize_t) (SIZE_MAX / 2)) #endif /* The type of indexes into strings. This is signed, not size_t, since the API requires indexes to fit in regoff_t anyway, and using signed integers makes the code a bit smaller and presumably faster. The traditional GNU regex implementation uses int for indexes. The POSIX-compatible implementation uses a possibly-wider type. The name 'Idx' is three letters to minimize the hassle of reindenting a lot of regex code that formerly used 'int'. */ typedef regoff_t Idx; #ifdef _REGEX_LARGE_OFFSETS # define IDX_MAX SSIZE_MAX #else # define IDX_MAX INT_MAX #endif /* A hash value, suitable for computing hash tables. */ typedef __re_size_t re_hashval_t; /* An integer used to represent a set of bits. It must be unsigned, and must be at least as wide as unsigned int. */ typedef unsigned long int bitset_word_t; /* All bits set in a bitset_word_t. */ #define BITSET_WORD_MAX ULONG_MAX /* Number of bits in a bitset_word_t. For portability to hosts with padding bits, do not use '(sizeof (bitset_word_t) * CHAR_BIT)'; instead, deduce it directly from BITSET_WORD_MAX. Avoid greater-than-32-bit integers and unconditional shifts by more than 31 bits, as they're not portable. */ #if BITSET_WORD_MAX == 0xffffffffUL # define BITSET_WORD_BITS 32 #elif BITSET_WORD_MAX >> 31 >> 4 == 1 # define BITSET_WORD_BITS 36 #elif BITSET_WORD_MAX >> 31 >> 16 == 1 # define BITSET_WORD_BITS 48 #elif BITSET_WORD_MAX >> 31 >> 28 == 1 # define BITSET_WORD_BITS 60 #elif BITSET_WORD_MAX >> 31 >> 31 >> 1 == 1 # define BITSET_WORD_BITS 64 #elif BITSET_WORD_MAX >> 31 >> 31 >> 9 == 1 # define BITSET_WORD_BITS 72 #elif BITSET_WORD_MAX >> 31 >> 31 >> 31 >> 31 >> 3 == 1 # define BITSET_WORD_BITS 128 #elif BITSET_WORD_MAX >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 7 == 1 # define BITSET_WORD_BITS 256 #elif BITSET_WORD_MAX >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 31 >> 7 > 1 # define BITSET_WORD_BITS 257 /* any value > SBC_MAX will do here */ # if BITSET_WORD_BITS <= SBC_MAX # error "Invalid SBC_MAX" # endif #else # error "Add case for new bitset_word_t size" #endif /* Number of bitset_word_t values in a bitset_t. */ #define BITSET_WORDS ((SBC_MAX + BITSET_WORD_BITS - 1) / BITSET_WORD_BITS) typedef bitset_word_t bitset_t[BITSET_WORDS]; typedef bitset_word_t *re_bitset_ptr_t; typedef const bitset_word_t *re_const_bitset_ptr_t; #define PREV_WORD_CONSTRAINT 0x0001 #define PREV_NOTWORD_CONSTRAINT 0x0002 #define NEXT_WORD_CONSTRAINT 0x0004 #define NEXT_NOTWORD_CONSTRAINT 0x0008 #define PREV_NEWLINE_CONSTRAINT 0x0010 #define NEXT_NEWLINE_CONSTRAINT 0x0020 #define PREV_BEGBUF_CONSTRAINT 0x0040 #define NEXT_ENDBUF_CONSTRAINT 0x0080 #define WORD_DELIM_CONSTRAINT 0x0100 #define NOT_WORD_DELIM_CONSTRAINT 0x0200 typedef enum { INSIDE_WORD = PREV_WORD_CONSTRAINT | NEXT_WORD_CONSTRAINT, WORD_FIRST = PREV_NOTWORD_CONSTRAINT | NEXT_WORD_CONSTRAINT, WORD_LAST = PREV_WORD_CONSTRAINT | NEXT_NOTWORD_CONSTRAINT, INSIDE_NOTWORD = PREV_NOTWORD_CONSTRAINT | NEXT_NOTWORD_CONSTRAINT, LINE_FIRST = PREV_NEWLINE_CONSTRAINT, LINE_LAST = NEXT_NEWLINE_CONSTRAINT, BUF_FIRST = PREV_BEGBUF_CONSTRAINT, BUF_LAST = NEXT_ENDBUF_CONSTRAINT, WORD_DELIM = WORD_DELIM_CONSTRAINT, NOT_WORD_DELIM = NOT_WORD_DELIM_CONSTRAINT } re_context_type; typedef struct { Idx alloc; Idx nelem; Idx *elems; } re_node_set; typedef enum { NON_TYPE = 0, /* Node type, These are used by token, node, tree. */ CHARACTER = 1, END_OF_RE = 2, SIMPLE_BRACKET = 3, OP_BACK_REF = 4, OP_PERIOD = 5, #ifdef RE_ENABLE_I18N COMPLEX_BRACKET = 6, OP_UTF8_PERIOD = 7, #endif /* RE_ENABLE_I18N */ /* We define EPSILON_BIT as a macro so that OP_OPEN_SUBEXP is used when the debugger shows values of this enum type. */ #define EPSILON_BIT 8 OP_OPEN_SUBEXP = EPSILON_BIT | 0, OP_CLOSE_SUBEXP = EPSILON_BIT | 1, OP_ALT = EPSILON_BIT | 2, OP_DUP_ASTERISK = EPSILON_BIT | 3, ANCHOR = EPSILON_BIT | 4, /* Tree type, these are used only by tree. */ CONCAT = 16, SUBEXP = 17, /* Token type, these are used only by token. */ OP_DUP_PLUS = 18, OP_DUP_QUESTION, OP_OPEN_BRACKET, OP_CLOSE_BRACKET, OP_CHARSET_RANGE, OP_OPEN_DUP_NUM, OP_CLOSE_DUP_NUM, OP_NON_MATCH_LIST, OP_OPEN_COLL_ELEM, OP_CLOSE_COLL_ELEM, OP_OPEN_EQUIV_CLASS, OP_CLOSE_EQUIV_CLASS, OP_OPEN_CHAR_CLASS, OP_CLOSE_CHAR_CLASS, OP_WORD, OP_NOTWORD, OP_SPACE, OP_NOTSPACE, BACK_SLASH } re_token_type_t; #ifdef RE_ENABLE_I18N typedef struct { /* Multibyte characters. */ wchar_t *mbchars; /* Collating symbols. */ # ifdef _LIBC int32_t *coll_syms; # endif /* Equivalence classes. */ # ifdef _LIBC int32_t *equiv_classes; # endif /* Range expressions. */ # ifdef _LIBC uint32_t *range_starts; uint32_t *range_ends; # else /* not _LIBC */ wchar_t *range_starts; wchar_t *range_ends; # endif /* not _LIBC */ /* Character classes. */ wctype_t *char_classes; /* If this character set is the non-matching list. */ unsigned int non_match : 1; /* # of multibyte characters. */ Idx nmbchars; /* # of collating symbols. */ Idx ncoll_syms; /* # of equivalence classes. */ Idx nequiv_classes; /* # of range expressions. */ Idx nranges; /* # of character classes. */ Idx nchar_classes; } re_charset_t; #endif /* RE_ENABLE_I18N */ typedef struct { union { unsigned char c; /* for CHARACTER */ re_bitset_ptr_t sbcset; /* for SIMPLE_BRACKET */ #ifdef RE_ENABLE_I18N re_charset_t *mbcset; /* for COMPLEX_BRACKET */ #endif /* RE_ENABLE_I18N */ Idx idx; /* for BACK_REF */ re_context_type ctx_type; /* for ANCHOR */ } opr; #if __GNUC__ >= 2 && !defined __STRICT_ANSI__ re_token_type_t type : 8; #else re_token_type_t type; #endif unsigned int constraint : 10; /* context constraint */ unsigned int duplicated : 1; unsigned int opt_subexp : 1; #ifdef RE_ENABLE_I18N unsigned int accept_mb : 1; /* These 2 bits can be moved into the union if needed (e.g. if running out of bits; move opr.c to opr.c.c and move the flags to opr.c.flags). */ unsigned int mb_partial : 1; #endif unsigned int word_char : 1; } re_token_t; #define IS_EPSILON_NODE(type) ((type) & EPSILON_BIT) struct re_string_t { /* Indicate the raw buffer which is the original string passed as an argument of regexec(), re_search(), etc.. */ const unsigned char *raw_mbs; /* Store the multibyte string. In case of "case insensitive mode" like REG_ICASE, upper cases of the string are stored, otherwise MBS points the same address that RAW_MBS points. */ unsigned char *mbs; #ifdef RE_ENABLE_I18N /* Store the wide character string which is corresponding to MBS. */ wint_t *wcs; Idx *offsets; mbstate_t cur_state; #endif /* Index in RAW_MBS. Each character mbs[i] corresponds to raw_mbs[raw_mbs_idx + i]. */ Idx raw_mbs_idx; /* The length of the valid characters in the buffers. */ Idx valid_len; /* The corresponding number of bytes in raw_mbs array. */ Idx valid_raw_len; /* The length of the buffers MBS and WCS. */ Idx bufs_len; /* The index in MBS, which is updated by re_string_fetch_byte. */ Idx cur_idx; /* length of RAW_MBS array. */ Idx raw_len; /* This is RAW_LEN - RAW_MBS_IDX + VALID_LEN - VALID_RAW_LEN. */ Idx len; /* End of the buffer may be shorter than its length in the cases such as re_match_2, re_search_2. Then, we use STOP for end of the buffer instead of LEN. */ Idx raw_stop; /* This is RAW_STOP - RAW_MBS_IDX adjusted through OFFSETS. */ Idx stop; /* The context of mbs[0]. We store the context independently, since the context of mbs[0] may be different from raw_mbs[0], which is the beginning of the input string. */ unsigned int tip_context; /* The translation passed as a part of an argument of re_compile_pattern. */ RE_TRANSLATE_TYPE trans; /* Copy of re_dfa_t's word_char. */ re_const_bitset_ptr_t word_char; /* true if REG_ICASE. */ unsigned char icase; unsigned char is_utf8; unsigned char map_notascii; unsigned char mbs_allocated; unsigned char offsets_needed; unsigned char newline_anchor; unsigned char word_ops_used; int mb_cur_max; }; typedef struct re_string_t re_string_t; struct re_dfa_t; typedef struct re_dfa_t re_dfa_t; #ifndef _LIBC # define IS_IN(libc) false #endif static reg_errcode_t re_string_realloc_buffers (re_string_t *pstr, Idx new_buf_len); #ifdef RE_ENABLE_I18N static void build_wcs_buffer (re_string_t *pstr); static reg_errcode_t build_wcs_upper_buffer (re_string_t *pstr); #endif /* RE_ENABLE_I18N */ static void build_upper_buffer (re_string_t *pstr); static void re_string_translate_buffer (re_string_t *pstr); static unsigned int re_string_context_at (const re_string_t *input, Idx idx, int eflags) __attribute__ ((pure)); #define re_string_peek_byte(pstr, offset) \ ((pstr)->mbs[(pstr)->cur_idx + offset]) #define re_string_fetch_byte(pstr) \ ((pstr)->mbs[(pstr)->cur_idx++]) #define re_string_first_byte(pstr, idx) \ ((idx) == (pstr)->valid_len || (pstr)->wcs[idx] != WEOF) #define re_string_is_single_byte_char(pstr, idx) \ ((pstr)->wcs[idx] != WEOF && ((pstr)->valid_len == (idx) + 1 \ || (pstr)->wcs[(idx) + 1] != WEOF)) #define re_string_eoi(pstr) ((pstr)->stop <= (pstr)->cur_idx) #define re_string_cur_idx(pstr) ((pstr)->cur_idx) #define re_string_get_buffer(pstr) ((pstr)->mbs) #define re_string_length(pstr) ((pstr)->len) #define re_string_byte_at(pstr,idx) ((pstr)->mbs[idx]) #define re_string_skip_bytes(pstr,idx) ((pstr)->cur_idx += (idx)) #define re_string_set_index(pstr,idx) ((pstr)->cur_idx = (idx)) #if defined _LIBC || HAVE_ALLOCA # include #endif #ifndef _LIBC # if HAVE_ALLOCA /* The OS usually guarantees only one guard page at the bottom of the stack, and a page size can be as small as 4096 bytes. So we cannot safely allocate anything larger than 4096 bytes. Also care for the possibility of a few compiler-allocated temporary stack slots. */ # define __libc_use_alloca(n) ((n) < 4032) # else /* alloca is implemented with malloc, so just use malloc. */ # define __libc_use_alloca(n) 0 # undef alloca # define alloca(n) malloc (n) # endif #endif #ifdef _LIBC # define MALLOC_0_IS_NONNULL 1 #elif !defined MALLOC_0_IS_NONNULL # define MALLOC_0_IS_NONNULL 0 #endif #ifndef MAX # define MAX(a,b) ((a) < (b) ? (b) : (a)) #endif #ifndef MIN # define MIN(a,b) ((a) < (b) ? (a) : (b)) #endif #define re_malloc(t,n) ((t *) malloc ((n) * sizeof (t))) #define re_realloc(p,t,n) ((t *) realloc (p, (n) * sizeof (t))) #define re_free(p) free (p) struct bin_tree_t { struct bin_tree_t *parent; struct bin_tree_t *left; struct bin_tree_t *right; struct bin_tree_t *first; struct bin_tree_t *next; re_token_t token; /* 'node_idx' is the index in dfa->nodes, if 'type' == 0. Otherwise 'type' indicate the type of this node. */ Idx node_idx; }; typedef struct bin_tree_t bin_tree_t; #define BIN_TREE_STORAGE_SIZE \ ((1024 - sizeof (void *)) / sizeof (bin_tree_t)) struct bin_tree_storage_t { struct bin_tree_storage_t *next; bin_tree_t data[BIN_TREE_STORAGE_SIZE]; }; typedef struct bin_tree_storage_t bin_tree_storage_t; #define CONTEXT_WORD 1 #define CONTEXT_NEWLINE (CONTEXT_WORD << 1) #define CONTEXT_BEGBUF (CONTEXT_NEWLINE << 1) #define CONTEXT_ENDBUF (CONTEXT_BEGBUF << 1) #define IS_WORD_CONTEXT(c) ((c) & CONTEXT_WORD) #define IS_NEWLINE_CONTEXT(c) ((c) & CONTEXT_NEWLINE) #define IS_BEGBUF_CONTEXT(c) ((c) & CONTEXT_BEGBUF) #define IS_ENDBUF_CONTEXT(c) ((c) & CONTEXT_ENDBUF) #define IS_ORDINARY_CONTEXT(c) ((c) == 0) #define IS_WORD_CHAR(ch) (isalnum (ch) || (ch) == '_') #define IS_NEWLINE(ch) ((ch) == NEWLINE_CHAR) #define IS_WIDE_WORD_CHAR(ch) (__iswalnum (ch) || (ch) == L'_') #define IS_WIDE_NEWLINE(ch) ((ch) == WIDE_NEWLINE_CHAR) #define NOT_SATISFY_PREV_CONSTRAINT(constraint,context) \ ((((constraint) & PREV_WORD_CONSTRAINT) && !IS_WORD_CONTEXT (context)) \ || ((constraint & PREV_NOTWORD_CONSTRAINT) && IS_WORD_CONTEXT (context)) \ || ((constraint & PREV_NEWLINE_CONSTRAINT) && !IS_NEWLINE_CONTEXT (context))\ || ((constraint & PREV_BEGBUF_CONSTRAINT) && !IS_BEGBUF_CONTEXT (context))) #define NOT_SATISFY_NEXT_CONSTRAINT(constraint,context) \ ((((constraint) & NEXT_WORD_CONSTRAINT) && !IS_WORD_CONTEXT (context)) \ || (((constraint) & NEXT_NOTWORD_CONSTRAINT) && IS_WORD_CONTEXT (context)) \ || (((constraint) & NEXT_NEWLINE_CONSTRAINT) && !IS_NEWLINE_CONTEXT (context)) \ || (((constraint) & NEXT_ENDBUF_CONSTRAINT) && !IS_ENDBUF_CONTEXT (context))) struct re_dfastate_t { re_hashval_t hash; re_node_set nodes; re_node_set non_eps_nodes; re_node_set inveclosure; re_node_set *entrance_nodes; struct re_dfastate_t **trtable, **word_trtable; unsigned int context : 4; unsigned int halt : 1; /* If this state can accept "multi byte". Note that we refer to multibyte characters, and multi character collating elements as "multi byte". */ unsigned int accept_mb : 1; /* If this state has backreference node(s). */ unsigned int has_backref : 1; unsigned int has_constraint : 1; }; typedef struct re_dfastate_t re_dfastate_t; struct re_state_table_entry { Idx num; Idx alloc; re_dfastate_t **array; }; /* Array type used in re_sub_match_last_t and re_sub_match_top_t. */ typedef struct { Idx next_idx; Idx alloc; re_dfastate_t **array; } state_array_t; /* Store information about the node NODE whose type is OP_CLOSE_SUBEXP. */ typedef struct { Idx node; Idx str_idx; /* The position NODE match at. */ state_array_t path; } re_sub_match_last_t; /* Store information about the node NODE whose type is OP_OPEN_SUBEXP. And information about the node, whose type is OP_CLOSE_SUBEXP, corresponding to NODE is stored in LASTS. */ typedef struct { Idx str_idx; Idx node; state_array_t *path; Idx alasts; /* Allocation size of LASTS. */ Idx nlasts; /* The number of LASTS. */ re_sub_match_last_t **lasts; } re_sub_match_top_t; struct re_backref_cache_entry { Idx node; Idx str_idx; Idx subexp_from; Idx subexp_to; char more; char unused; unsigned short int eps_reachable_subexps_map; }; typedef struct { /* The string object corresponding to the input string. */ re_string_t input; #if defined _LIBC || (defined __STDC_VERSION__ && __STDC_VERSION__ >= 199901L) const re_dfa_t *const dfa; #else const re_dfa_t *dfa; #endif /* EFLAGS of the argument of regexec. */ int eflags; /* Where the matching ends. */ Idx match_last; Idx last_node; /* The state log used by the matcher. */ re_dfastate_t **state_log; Idx state_log_top; /* Back reference cache. */ Idx nbkref_ents; Idx abkref_ents; struct re_backref_cache_entry *bkref_ents; int max_mb_elem_len; Idx nsub_tops; Idx asub_tops; re_sub_match_top_t **sub_tops; } re_match_context_t; typedef struct { re_dfastate_t **sifted_states; re_dfastate_t **limited_states; Idx last_node; Idx last_str_idx; re_node_set limits; } re_sift_context_t; struct re_fail_stack_ent_t { Idx idx; Idx node; regmatch_t *regs; re_node_set eps_via_nodes; }; struct re_fail_stack_t { Idx num; Idx alloc; struct re_fail_stack_ent_t *stack; }; struct re_dfa_t { re_token_t *nodes; size_t nodes_alloc; size_t nodes_len; Idx *nexts; Idx *org_indices; re_node_set *edests; re_node_set *eclosures; re_node_set *inveclosures; struct re_state_table_entry *state_table; re_dfastate_t *init_state; re_dfastate_t *init_state_word; re_dfastate_t *init_state_nl; re_dfastate_t *init_state_begbuf; bin_tree_t *str_tree; bin_tree_storage_t *str_tree_storage; re_bitset_ptr_t sb_char; int str_tree_storage_idx; /* number of subexpressions 're_nsub' is in regex_t. */ re_hashval_t state_hash_mask; Idx init_node; Idx nbackref; /* The number of backreference in this dfa. */ /* Bitmap expressing which backreference is used. */ bitset_word_t used_bkref_map; bitset_word_t completed_bkref_map; unsigned int has_plural_match : 1; /* If this dfa has "multibyte node", which is a backreference or a node which can accept multibyte character or multi character collating element. */ unsigned int has_mb_node : 1; unsigned int is_utf8 : 1; unsigned int map_notascii : 1; unsigned int word_ops_used : 1; int mb_cur_max; bitset_t word_char; reg_syntax_t syntax; Idx *subexp_map; #ifdef DEBUG char* re_str; #endif lock_define (lock) }; #define re_node_set_init_empty(set) memset (set, '\0', sizeof (re_node_set)) #define re_node_set_remove(set,id) \ (re_node_set_remove_at (set, re_node_set_contains (set, id) - 1)) #define re_node_set_empty(p) ((p)->nelem = 0) #define re_node_set_free(set) re_free ((set)->elems) typedef enum { SB_CHAR, MB_CHAR, EQUIV_CLASS, COLL_SYM, CHAR_CLASS } bracket_elem_type; typedef struct { bracket_elem_type type; union { unsigned char ch; unsigned char *name; wchar_t wch; } opr; } bracket_elem_t; /* Functions for bitset_t operation. */ static void bitset_set (bitset_t set, Idx i) { set[i / BITSET_WORD_BITS] |= (bitset_word_t) 1 << i % BITSET_WORD_BITS; } static void bitset_clear (bitset_t set, Idx i) { set[i / BITSET_WORD_BITS] &= ~ ((bitset_word_t) 1 << i % BITSET_WORD_BITS); } static bool bitset_contain (const bitset_t set, Idx i) { return (set[i / BITSET_WORD_BITS] >> i % BITSET_WORD_BITS) & 1; } static void bitset_empty (bitset_t set) { memset (set, '\0', sizeof (bitset_t)); } static void bitset_set_all (bitset_t set) { memset (set, -1, sizeof (bitset_word_t) * (SBC_MAX / BITSET_WORD_BITS)); if (SBC_MAX % BITSET_WORD_BITS != 0) set[BITSET_WORDS - 1] = ((bitset_word_t) 1 << SBC_MAX % BITSET_WORD_BITS) - 1; } static void bitset_copy (bitset_t dest, const bitset_t src) { memcpy (dest, src, sizeof (bitset_t)); } static void __attribute__ ((unused)) bitset_not (bitset_t set) { int bitset_i; for (bitset_i = 0; bitset_i < SBC_MAX / BITSET_WORD_BITS; ++bitset_i) set[bitset_i] = ~set[bitset_i]; if (SBC_MAX % BITSET_WORD_BITS != 0) set[BITSET_WORDS - 1] = ((((bitset_word_t) 1 << SBC_MAX % BITSET_WORD_BITS) - 1) & ~set[BITSET_WORDS - 1]); } static void __attribute__ ((unused)) bitset_merge (bitset_t dest, const bitset_t src) { int bitset_i; for (bitset_i = 0; bitset_i < BITSET_WORDS; ++bitset_i) dest[bitset_i] |= src[bitset_i]; } static void __attribute__ ((unused)) bitset_mask (bitset_t dest, const bitset_t src) { int bitset_i; for (bitset_i = 0; bitset_i < BITSET_WORDS; ++bitset_i) dest[bitset_i] &= src[bitset_i]; } #ifdef RE_ENABLE_I18N /* Functions for re_string. */ static int __attribute__ ((pure, unused)) re_string_char_size_at (const re_string_t *pstr, Idx idx) { int byte_idx; if (pstr->mb_cur_max == 1) return 1; for (byte_idx = 1; idx + byte_idx < pstr->valid_len; ++byte_idx) if (pstr->wcs[idx + byte_idx] != WEOF) break; return byte_idx; } static wint_t __attribute__ ((pure, unused)) re_string_wchar_at (const re_string_t *pstr, Idx idx) { if (pstr->mb_cur_max == 1) return (wint_t) pstr->mbs[idx]; return (wint_t) pstr->wcs[idx]; } # ifdef _LIBC # include # endif static int __attribute__ ((pure, unused)) re_string_elem_size_at (const re_string_t *pstr, Idx idx) { # ifdef _LIBC const unsigned char *p, *extra; const int32_t *table, *indirect; uint_fast32_t nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules != 0) { table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_EXTRAMB); indirect = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_INDIRECTMB); p = pstr->mbs + idx; findidx (table, indirect, extra, &p, pstr->len - idx); return p - pstr->mbs - idx; } else # endif /* _LIBC */ return 1; } #endif /* RE_ENABLE_I18N */ #ifndef __GNUC_PREREQ # if defined __GNUC__ && defined __GNUC_MINOR__ # define __GNUC_PREREQ(maj, min) \ ((__GNUC__ << 16) + __GNUC_MINOR__ >= ((maj) << 16) + (min)) # else # define __GNUC_PREREQ(maj, min) 0 # endif #endif #if __GNUC_PREREQ (3,4) # undef __attribute_warn_unused_result__ # define __attribute_warn_unused_result__ \ __attribute__ ((__warn_unused_result__)) #else # define __attribute_warn_unused_result__ /* empty */ #endif #ifndef FALLTHROUGH # if __GNUC__ < 7 # define FALLTHROUGH ((void) 0) # else # define FALLTHROUGH __attribute__ ((__fallthrough__)) # endif #endif #endif /* _REGEX_INTERNAL_H */ gnuastro-0.5/bootstrapped/lib/regex.h0000644000175000017500000006013513217200021014671 00000000000000/* Definitions for data structures and routines for the regular expression library. Copyright (C) 1985, 1989-1993, 1995-1998, 2000-2003, 2005-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _REGEX_H #define _REGEX_H 1 #include /* Allow the use in C++ code. */ #ifdef __cplusplus extern "C" { #endif /* Define __USE_GNU to declare GNU extensions that violate the POSIX name space rules. */ #ifdef _GNU_SOURCE # define __USE_GNU 1 #endif #ifdef _REGEX_LARGE_OFFSETS /* Use types and values that are wide enough to represent signed and unsigned byte offsets in memory. This currently works only when the regex code is used outside of the GNU C library; it is not yet supported within glibc itself, and glibc users should not define _REGEX_LARGE_OFFSETS. */ /* The type of object sizes. */ typedef size_t __re_size_t; /* The type of object sizes, in places where the traditional code uses unsigned long int. */ typedef size_t __re_long_size_t; #else /* The traditional GNU regex implementation mishandles strings longer than INT_MAX. */ typedef unsigned int __re_size_t; typedef unsigned long int __re_long_size_t; #endif /* The following two types have to be signed and unsigned integer type wide enough to hold a value of a pointer. For most ANSI compilers ptrdiff_t and size_t should be likely OK. Still size of these two types is 2 for Microsoft C. Ugh... */ typedef long int s_reg_t; typedef unsigned long int active_reg_t; /* The following bits are used to determine the regexp syntax we recognize. The set/not-set meanings are chosen so that Emacs syntax remains the value 0. The bits are given in alphabetical order, and the definitions shifted by one from the previous bit; thus, when we add or remove a bit, only one other definition need change. */ typedef unsigned long int reg_syntax_t; #ifdef __USE_GNU /* If this bit is not set, then \ inside a bracket expression is literal. If set, then such a \ quotes the following character. */ # define RE_BACKSLASH_ESCAPE_IN_LISTS ((unsigned long int) 1) /* If this bit is not set, then + and ? are operators, and \+ and \? are literals. If set, then \+ and \? are operators and + and ? are literals. */ # define RE_BK_PLUS_QM (RE_BACKSLASH_ESCAPE_IN_LISTS << 1) /* If this bit is set, then character classes are supported. They are: [:alpha:], [:upper:], [:lower:], [:digit:], [:alnum:], [:xdigit:], [:space:], [:print:], [:punct:], [:graph:], and [:cntrl:]. If not set, then character classes are not supported. */ # define RE_CHAR_CLASSES (RE_BK_PLUS_QM << 1) /* If this bit is set, then ^ and $ are always anchors (outside bracket expressions, of course). If this bit is not set, then it depends: ^ is an anchor if it is at the beginning of a regular expression or after an open-group or an alternation operator; $ is an anchor if it is at the end of a regular expression, or before a close-group or an alternation operator. This bit could be (re)combined with RE_CONTEXT_INDEP_OPS, because POSIX draft 11.2 says that * etc. in leading positions is undefined. We already implemented a previous draft which made those constructs invalid, though, so we haven't changed the code back. */ # define RE_CONTEXT_INDEP_ANCHORS (RE_CHAR_CLASSES << 1) /* If this bit is set, then special characters are always special regardless of where they are in the pattern. If this bit is not set, then special characters are special only in some contexts; otherwise they are ordinary. Specifically, * + ? and intervals are only special when not after the beginning, open-group, or alternation operator. */ # define RE_CONTEXT_INDEP_OPS (RE_CONTEXT_INDEP_ANCHORS << 1) /* If this bit is set, then *, +, ?, and { cannot be first in an re or immediately after an alternation or begin-group operator. */ # define RE_CONTEXT_INVALID_OPS (RE_CONTEXT_INDEP_OPS << 1) /* If this bit is set, then . matches newline. If not set, then it doesn't. */ # define RE_DOT_NEWLINE (RE_CONTEXT_INVALID_OPS << 1) /* If this bit is set, then . doesn't match NUL. If not set, then it does. */ # define RE_DOT_NOT_NULL (RE_DOT_NEWLINE << 1) /* If this bit is set, nonmatching lists [^...] do not match newline. If not set, they do. */ # define RE_HAT_LISTS_NOT_NEWLINE (RE_DOT_NOT_NULL << 1) /* If this bit is set, either \{...\} or {...} defines an interval, depending on RE_NO_BK_BRACES. If not set, \{, \}, {, and } are literals. */ # define RE_INTERVALS (RE_HAT_LISTS_NOT_NEWLINE << 1) /* If this bit is set, +, ? and | aren't recognized as operators. If not set, they are. */ # define RE_LIMITED_OPS (RE_INTERVALS << 1) /* If this bit is set, newline is an alternation operator. If not set, newline is literal. */ # define RE_NEWLINE_ALT (RE_LIMITED_OPS << 1) /* If this bit is set, then '{...}' defines an interval, and \{ and \} are literals. If not set, then '\{...\}' defines an interval. */ # define RE_NO_BK_BRACES (RE_NEWLINE_ALT << 1) /* If this bit is set, (...) defines a group, and \( and \) are literals. If not set, \(...\) defines a group, and ( and ) are literals. */ # define RE_NO_BK_PARENS (RE_NO_BK_BRACES << 1) /* If this bit is set, then \ matches . If not set, then \ is a back-reference. */ # define RE_NO_BK_REFS (RE_NO_BK_PARENS << 1) /* If this bit is set, then | is an alternation operator, and \| is literal. If not set, then \| is an alternation operator, and | is literal. */ # define RE_NO_BK_VBAR (RE_NO_BK_REFS << 1) /* If this bit is set, then an ending range point collating higher than the starting range point, as in [z-a], is invalid. If not set, then when ending range point collates higher than the starting range point, the range is ignored. */ # define RE_NO_EMPTY_RANGES (RE_NO_BK_VBAR << 1) /* If this bit is set, then an unmatched ) is ordinary. If not set, then an unmatched ) is invalid. */ # define RE_UNMATCHED_RIGHT_PAREN_ORD (RE_NO_EMPTY_RANGES << 1) /* If this bit is set, succeed as soon as we match the whole pattern, without further backtracking. */ # define RE_NO_POSIX_BACKTRACKING (RE_UNMATCHED_RIGHT_PAREN_ORD << 1) /* If this bit is set, do not process the GNU regex operators. If not set, then the GNU regex operators are recognized. */ # define RE_NO_GNU_OPS (RE_NO_POSIX_BACKTRACKING << 1) /* If this bit is set, turn on internal regex debugging. If not set, and debugging was on, turn it off. This only works if regex.c is compiled -DDEBUG. We define this bit always, so that all that's needed to turn on debugging is to recompile regex.c; the calling code can always have this bit set, and it won't affect anything in the normal case. */ # define RE_DEBUG (RE_NO_GNU_OPS << 1) /* If this bit is set, a syntactically invalid interval is treated as a string of ordinary characters. For example, the ERE 'a{1' is treated as 'a\{1'. */ # define RE_INVALID_INTERVAL_ORD (RE_DEBUG << 1) /* If this bit is set, then ignore case when matching. If not set, then case is significant. */ # define RE_ICASE (RE_INVALID_INTERVAL_ORD << 1) /* This bit is used internally like RE_CONTEXT_INDEP_ANCHORS but only for ^, because it is difficult to scan the regex backwards to find whether ^ should be special. */ # define RE_CARET_ANCHORS_HERE (RE_ICASE << 1) /* If this bit is set, then \{ cannot be first in a regex or immediately after an alternation, open-group or \} operator. */ # define RE_CONTEXT_INVALID_DUP (RE_CARET_ANCHORS_HERE << 1) /* If this bit is set, then no_sub will be set to 1 during re_compile_pattern. */ # define RE_NO_SUB (RE_CONTEXT_INVALID_DUP << 1) #endif /* This global variable defines the particular regexp syntax to use (for some interfaces). When a regexp is compiled, the syntax used is stored in the pattern buffer, so changing this does not affect already-compiled regexps. */ extern reg_syntax_t re_syntax_options; #ifdef __USE_GNU /* Define combinations of the above bits for the standard possibilities. (The [[[ comments delimit what gets put into the Texinfo file, so don't delete them!) */ /* [[[begin syntaxes]]] */ # define RE_SYNTAX_EMACS 0 # define RE_SYNTAX_AWK \ (RE_BACKSLASH_ESCAPE_IN_LISTS | RE_DOT_NOT_NULL \ | RE_NO_BK_PARENS | RE_NO_BK_REFS \ | RE_NO_BK_VBAR | RE_NO_EMPTY_RANGES \ | RE_DOT_NEWLINE | RE_CONTEXT_INDEP_ANCHORS \ | RE_CHAR_CLASSES \ | RE_UNMATCHED_RIGHT_PAREN_ORD | RE_NO_GNU_OPS) # define RE_SYNTAX_GNU_AWK \ ((RE_SYNTAX_POSIX_EXTENDED | RE_BACKSLASH_ESCAPE_IN_LISTS \ | RE_INVALID_INTERVAL_ORD) \ & ~(RE_DOT_NOT_NULL | RE_CONTEXT_INDEP_OPS \ | RE_CONTEXT_INVALID_OPS )) # define RE_SYNTAX_POSIX_AWK \ (RE_SYNTAX_POSIX_EXTENDED | RE_BACKSLASH_ESCAPE_IN_LISTS \ | RE_INTERVALS | RE_NO_GNU_OPS \ | RE_INVALID_INTERVAL_ORD) # define RE_SYNTAX_GREP \ ((RE_SYNTAX_POSIX_BASIC | RE_NEWLINE_ALT) \ & ~(RE_CONTEXT_INVALID_DUP | RE_DOT_NOT_NULL)) # define RE_SYNTAX_EGREP \ ((RE_SYNTAX_POSIX_EXTENDED | RE_INVALID_INTERVAL_ORD | RE_NEWLINE_ALT) \ & ~(RE_CONTEXT_INVALID_OPS | RE_DOT_NOT_NULL)) /* POSIX grep -E behavior is no longer incompatible with GNU. */ # define RE_SYNTAX_POSIX_EGREP \ RE_SYNTAX_EGREP /* P1003.2/D11.2, section 4.20.7.1, lines 5078ff. */ # define RE_SYNTAX_ED RE_SYNTAX_POSIX_BASIC # define RE_SYNTAX_SED RE_SYNTAX_POSIX_BASIC /* Syntax bits common to both basic and extended POSIX regex syntax. */ # define _RE_SYNTAX_POSIX_COMMON \ (RE_CHAR_CLASSES | RE_DOT_NEWLINE | RE_DOT_NOT_NULL \ | RE_INTERVALS | RE_NO_EMPTY_RANGES) # define RE_SYNTAX_POSIX_BASIC \ (_RE_SYNTAX_POSIX_COMMON | RE_BK_PLUS_QM | RE_CONTEXT_INVALID_DUP) /* Differs from ..._POSIX_BASIC only in that RE_BK_PLUS_QM becomes RE_LIMITED_OPS, i.e., \? \+ \| are not recognized. Actually, this isn't minimal, since other operators, such as \`, aren't disabled. */ # define RE_SYNTAX_POSIX_MINIMAL_BASIC \ (_RE_SYNTAX_POSIX_COMMON | RE_LIMITED_OPS) # define RE_SYNTAX_POSIX_EXTENDED \ (_RE_SYNTAX_POSIX_COMMON | RE_CONTEXT_INDEP_ANCHORS \ | RE_CONTEXT_INDEP_OPS | RE_NO_BK_BRACES \ | RE_NO_BK_PARENS | RE_NO_BK_VBAR \ | RE_CONTEXT_INVALID_OPS | RE_UNMATCHED_RIGHT_PAREN_ORD) /* Differs from ..._POSIX_EXTENDED in that RE_CONTEXT_INDEP_OPS is removed and RE_NO_BK_REFS is added. */ # define RE_SYNTAX_POSIX_MINIMAL_EXTENDED \ (_RE_SYNTAX_POSIX_COMMON | RE_CONTEXT_INDEP_ANCHORS \ | RE_CONTEXT_INVALID_OPS | RE_NO_BK_BRACES \ | RE_NO_BK_PARENS | RE_NO_BK_REFS \ | RE_NO_BK_VBAR | RE_UNMATCHED_RIGHT_PAREN_ORD) /* [[[end syntaxes]]] */ /* Maximum number of duplicates an interval can allow. POSIX-conforming systems might define this in , but we want our value, so remove any previous define. */ # ifdef _REGEX_INCLUDE_LIMITS_H # include # endif # ifdef RE_DUP_MAX # undef RE_DUP_MAX # endif /* RE_DUP_MAX is 2**15 - 1 because an earlier implementation stored the counter as a 2-byte signed integer. This is no longer true, so RE_DUP_MAX could be increased to (INT_MAX / 10 - 1), or to ((SIZE_MAX - 9) / 10) if _REGEX_LARGE_OFFSETS is defined. However, there would be a huge performance problem if someone actually used a pattern like a\{214748363\}, so RE_DUP_MAX retains its historical value. */ # define RE_DUP_MAX (0x7fff) #endif /* POSIX 'cflags' bits (i.e., information for 'regcomp'). */ /* If this bit is set, then use extended regular expression syntax. If not set, then use basic regular expression syntax. */ #define REG_EXTENDED 1 /* If this bit is set, then ignore case when matching. If not set, then case is significant. */ #define REG_ICASE (1 << 1) /* If this bit is set, then anchors do not match at newline characters in the string. If not set, then anchors do match at newlines. */ #define REG_NEWLINE (1 << 2) /* If this bit is set, then report only success or fail in regexec. If not set, then returns differ between not matching and errors. */ #define REG_NOSUB (1 << 3) /* POSIX 'eflags' bits (i.e., information for regexec). */ /* If this bit is set, then the beginning-of-line operator doesn't match the beginning of the string (presumably because it's not the beginning of a line). If not set, then the beginning-of-line operator does match the beginning of the string. */ #define REG_NOTBOL 1 /* Like REG_NOTBOL, except for the end-of-line. */ #define REG_NOTEOL (1 << 1) /* Use PMATCH[0] to delimit the start and end of the search in the buffer. */ #define REG_STARTEND (1 << 2) /* If any error codes are removed, changed, or added, update the '__re_error_msgid' table in regcomp.c. */ typedef enum { _REG_ENOSYS = -1, /* This will never happen for this implementation. */ _REG_NOERROR = 0, /* Success. */ _REG_NOMATCH, /* Didn't find a match (for regexec). */ /* POSIX regcomp return error codes. (In the order listed in the standard.) */ _REG_BADPAT, /* Invalid pattern. */ _REG_ECOLLATE, /* Invalid collating element. */ _REG_ECTYPE, /* Invalid character class name. */ _REG_EESCAPE, /* Trailing backslash. */ _REG_ESUBREG, /* Invalid back reference. */ _REG_EBRACK, /* Unmatched left bracket. */ _REG_EPAREN, /* Parenthesis imbalance. */ _REG_EBRACE, /* Unmatched \{. */ _REG_BADBR, /* Invalid contents of \{\}. */ _REG_ERANGE, /* Invalid range end. */ _REG_ESPACE, /* Ran out of memory. */ _REG_BADRPT, /* No preceding re for repetition op. */ /* Error codes we've added. */ _REG_EEND, /* Premature end. */ _REG_ESIZE, /* Too large (e.g., repeat count too large). */ _REG_ERPAREN /* Unmatched ) or \); not returned from regcomp. */ } reg_errcode_t; #if defined _XOPEN_SOURCE || defined __USE_XOPEN2K # define REG_ENOSYS _REG_ENOSYS #endif #define REG_NOERROR _REG_NOERROR #define REG_NOMATCH _REG_NOMATCH #define REG_BADPAT _REG_BADPAT #define REG_ECOLLATE _REG_ECOLLATE #define REG_ECTYPE _REG_ECTYPE #define REG_EESCAPE _REG_EESCAPE #define REG_ESUBREG _REG_ESUBREG #define REG_EBRACK _REG_EBRACK #define REG_EPAREN _REG_EPAREN #define REG_EBRACE _REG_EBRACE #define REG_BADBR _REG_BADBR #define REG_ERANGE _REG_ERANGE #define REG_ESPACE _REG_ESPACE #define REG_BADRPT _REG_BADRPT #define REG_EEND _REG_EEND #define REG_ESIZE _REG_ESIZE #define REG_ERPAREN _REG_ERPAREN /* This data structure represents a compiled pattern. Before calling the pattern compiler, the fields 'buffer', 'allocated', 'fastmap', and 'translate' can be set. After the pattern has been compiled, the fields 're_nsub', 'not_bol' and 'not_eol' are available. All other fields are private to the regex routines. */ #ifndef RE_TRANSLATE_TYPE # define __RE_TRANSLATE_TYPE unsigned char * # ifdef __USE_GNU # define RE_TRANSLATE_TYPE __RE_TRANSLATE_TYPE # endif #endif #ifdef __USE_GNU # define __REPB_PREFIX(name) name #else # define __REPB_PREFIX(name) __##name #endif struct re_pattern_buffer { /* Space that holds the compiled pattern. The type 'struct re_dfa_t' is private and is not declared here. */ struct re_dfa_t *__REPB_PREFIX(buffer); /* Number of bytes to which 'buffer' points. */ __re_long_size_t __REPB_PREFIX(allocated); /* Number of bytes actually used in 'buffer'. */ __re_long_size_t __REPB_PREFIX(used); /* Syntax setting with which the pattern was compiled. */ reg_syntax_t __REPB_PREFIX(syntax); /* Pointer to a fastmap, if any, otherwise zero. re_search uses the fastmap, if there is one, to skip over impossible starting points for matches. */ char *__REPB_PREFIX(fastmap); /* Either a translate table to apply to all characters before comparing them, or zero for no translation. The translation is applied to a pattern when it is compiled and to a string when it is matched. */ __RE_TRANSLATE_TYPE __REPB_PREFIX(translate); /* Number of subexpressions found by the compiler. */ size_t re_nsub; /* Zero if this pattern cannot match the empty string, one else. Well, in truth it's used only in 're_search_2', to see whether or not we should use the fastmap, so we don't set this absolutely perfectly; see 're_compile_fastmap' (the "duplicate" case). */ unsigned __REPB_PREFIX(can_be_null) : 1; /* If REGS_UNALLOCATED, allocate space in the 'regs' structure for 'max (RE_NREGS, re_nsub + 1)' groups. If REGS_REALLOCATE, reallocate space if necessary. If REGS_FIXED, use what's there. */ #ifdef __USE_GNU # define REGS_UNALLOCATED 0 # define REGS_REALLOCATE 1 # define REGS_FIXED 2 #endif unsigned __REPB_PREFIX(regs_allocated) : 2; /* Set to zero when 're_compile_pattern' compiles a pattern; set to one by 're_compile_fastmap' if it updates the fastmap. */ unsigned __REPB_PREFIX(fastmap_accurate) : 1; /* If set, 're_match_2' does not return information about subexpressions. */ unsigned __REPB_PREFIX(no_sub) : 1; /* If set, a beginning-of-line anchor doesn't match at the beginning of the string. */ unsigned __REPB_PREFIX(not_bol) : 1; /* Similarly for an end-of-line anchor. */ unsigned __REPB_PREFIX(not_eol) : 1; /* If true, an anchor at a newline matches. */ unsigned __REPB_PREFIX(newline_anchor) : 1; }; typedef struct re_pattern_buffer regex_t; /* Type for byte offsets within the string. POSIX mandates this. */ #ifdef _REGEX_LARGE_OFFSETS /* POSIX 1003.1-2008 requires that regoff_t be at least as wide as ptrdiff_t and ssize_t. We don't know of any hosts where ptrdiff_t is wider than ssize_t, so ssize_t is safe. ptrdiff_t is not visible here, so use ssize_t. */ typedef ssize_t regoff_t; #else /* The traditional GNU regex implementation mishandles strings longer than INT_MAX. */ typedef int regoff_t; #endif #ifdef __USE_GNU /* This is the structure we store register match data in. See regex.texinfo for a full description of what registers match. */ struct re_registers { __re_size_t num_regs; regoff_t *start; regoff_t *end; }; /* If 'regs_allocated' is REGS_UNALLOCATED in the pattern buffer, 're_match_2' returns information about at least this many registers the first time a 'regs' structure is passed. */ # ifndef RE_NREGS # define RE_NREGS 30 # endif #endif /* POSIX specification for registers. Aside from the different names than 're_registers', POSIX uses an array of structures, instead of a structure of arrays. */ typedef struct { regoff_t rm_so; /* Byte offset from string's start to substring's start. */ regoff_t rm_eo; /* Byte offset from string's start to substring's end. */ } regmatch_t; /* Declarations for routines. */ #ifdef __USE_GNU /* Sets the current default syntax to SYNTAX, and return the old syntax. You can also simply assign to the 're_syntax_options' variable. */ extern reg_syntax_t re_set_syntax (reg_syntax_t __syntax); /* Compile the regular expression PATTERN, with length LENGTH and syntax given by the global 're_syntax_options', into the buffer BUFFER. Return NULL if successful, and an error string if not. To free the allocated storage, you must call 'regfree' on BUFFER. Note that the translate table must either have been initialized by 'regcomp', with a malloc'ed value, or set to NULL before calling 'regfree'. */ extern const char *re_compile_pattern (const char *__pattern, size_t __length, struct re_pattern_buffer *__buffer); /* Compile a fastmap for the compiled pattern in BUFFER; used to accelerate searches. Return 0 if successful and -2 if was an internal error. */ extern int re_compile_fastmap (struct re_pattern_buffer *__buffer); /* Search in the string STRING (with length LENGTH) for the pattern compiled into BUFFER. Start searching at position START, for RANGE characters. Return the starting position of the match, -1 for no match, or -2 for an internal error. Also return register information in REGS (if REGS and BUFFER->no_sub are nonzero). */ extern regoff_t re_search (struct re_pattern_buffer *__buffer, const char *__String, regoff_t __length, regoff_t __start, regoff_t __range, struct re_registers *__regs); /* Like 're_search', but search in the concatenation of STRING1 and STRING2. Also, stop searching at index START + STOP. */ extern regoff_t re_search_2 (struct re_pattern_buffer *__buffer, const char *__string1, regoff_t __length1, const char *__string2, regoff_t __length2, regoff_t __start, regoff_t __range, struct re_registers *__regs, regoff_t __stop); /* Like 're_search', but return how many characters in STRING the regexp in BUFFER matched, starting at position START. */ extern regoff_t re_match (struct re_pattern_buffer *__buffer, const char *__String, regoff_t __length, regoff_t __start, struct re_registers *__regs); /* Relates to 're_match' as 're_search_2' relates to 're_search'. */ extern regoff_t re_match_2 (struct re_pattern_buffer *__buffer, const char *__string1, regoff_t __length1, const char *__string2, regoff_t __length2, regoff_t __start, struct re_registers *__regs, regoff_t __stop); /* Set REGS to hold NUM_REGS registers, storing them in STARTS and ENDS. Subsequent matches using BUFFER and REGS will use this memory for recording register information. STARTS and ENDS must be allocated with malloc, and must each be at least 'NUM_REGS * sizeof (regoff_t)' bytes long. If NUM_REGS == 0, then subsequent matches should allocate their own register data. Unless this function is called, the first search or match using BUFFER will allocate its own register data, without freeing the old data. */ extern void re_set_registers (struct re_pattern_buffer *__buffer, struct re_registers *__regs, __re_size_t __num_regs, regoff_t *__starts, regoff_t *__ends); #endif /* Use GNU */ #if defined _REGEX_RE_COMP || (defined _LIBC && defined __USE_MISC) # ifndef _CRAY /* 4.2 bsd compatibility. */ extern char *re_comp (const char *); extern int re_exec (const char *); # endif #endif /* GCC 2.95 and later have "__restrict"; C99 compilers have "restrict", and "configure" may have defined "restrict". Other compilers use __restrict, __restrict__, and _Restrict, and 'configure' might #define 'restrict' to those words, so pick a different name. */ #ifndef _Restrict_ # if 199901L <= __STDC_VERSION__ # define _Restrict_ restrict # elif 2 < __GNUC__ || (2 == __GNUC__ && 95 <= __GNUC_MINOR__) # define _Restrict_ __restrict # else # define _Restrict_ # endif #endif /* gcc 3.1 and up support the [restrict] syntax. Don't trust sys/cdefs.h's definition of __restrict_arr, though, as it mishandles gcc -ansi -pedantic. */ #ifndef _Restrict_arr_ # if ((199901L <= __STDC_VERSION__ \ || ((3 < __GNUC__ || (3 == __GNUC__ && 1 <= __GNUC_MINOR__)) \ && !defined __STRICT_ANSI__)) \ && !defined __GNUG__) # define _Restrict_arr_ _Restrict_ # else # define _Restrict_arr_ # endif #endif /* POSIX compatibility. */ extern int regcomp (regex_t *_Restrict_ __preg, const char *_Restrict_ __pattern, int __cflags); extern int regexec (const regex_t *_Restrict_ __preg, const char *_Restrict_ __String, size_t __nmatch, regmatch_t __pmatch[_Restrict_arr_], int __eflags); extern size_t regerror (int __errcode, const regex_t *_Restrict_ __preg, char *_Restrict_ __errbuf, size_t __errbuf_size); extern void regfree (regex_t *__preg); #ifdef __cplusplus } #endif /* C++ */ #endif /* regex.h */ gnuastro-0.5/bootstrapped/lib/rawmemchr.valgrind0000644000175000017500000000040313217200021017113 00000000000000# Suppress a valgrind message about use of uninitialized memory in rawmemchr(). # This use is OK because it provides only a speedup. { rawmemchr-value4 Memcheck:Value4 fun:rawmemchr } { rawmemchr-value8 Memcheck:Value8 fun:rawmemchr } gnuastro-0.5/bootstrapped/lib/nproc.h0000644000175000017500000000331213217200021014672 00000000000000/* Detect the number of processors. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Glen Lenker and Bruno Haible. */ /* Allow the use in C++ code. */ #ifdef __cplusplus extern "C" { #endif /* A "processor" in this context means a thread execution unit, that is either - an execution core in a (possibly multi-core) chip, in a (possibly multi- chip) module, in a single computer, or - a thread execution unit inside a core (hyper-threading, see ). Which of the two definitions is used, is unspecified. */ enum nproc_query { NPROC_ALL, /* total number of processors */ NPROC_CURRENT, /* processors available to the current process */ NPROC_CURRENT_OVERRIDABLE /* likewise, but overridable through the OMP_NUM_THREADS environment variable */ }; /* Return the total number of processors. The result is guaranteed to be at least 1. */ extern unsigned long int num_processors (enum nproc_query query); #ifdef __cplusplus } #endif /* C++ */ gnuastro-0.5/bootstrapped/lib/msvc-nothrow.h0000644000175000017500000000301113217200021016213 00000000000000/* Wrappers that don't throw invalid parameter notifications with MSVC runtime libraries. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MSVC_NOTHROW_H #define _MSVC_NOTHROW_H /* With MSVC runtime libraries with the "invalid parameter handler" concept, functions like fprintf(), dup2(), or close() crash when the caller passes an invalid argument. But POSIX wants error codes (such as EINVAL or EBADF) instead. This file defines wrappers that turn such an invalid parameter notification into an error code. */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get original declaration of _get_osfhandle. */ # include # if HAVE_MSVC_INVALID_PARAMETER_HANDLER /* Override _get_osfhandle. */ extern intptr_t _gl_nothrow_get_osfhandle (int fd); # define _get_osfhandle _gl_nothrow_get_osfhandle # endif #endif #endif /* _MSVC_NOTHROW_H */ gnuastro-0.5/bootstrapped/lib/msvc-inval.h0000644000175000017500000002114013217200021015627 00000000000000/* Invalid parameter handler for MSVC runtime libraries. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MSVC_INVAL_H #define _MSVC_INVAL_H /* With MSVC runtime libraries with the "invalid parameter handler" concept, functions like fprintf(), dup2(), or close() crash when the caller passes an invalid argument. But POSIX wants error codes (such as EINVAL or EBADF) instead. This file defines macros that turn such an invalid parameter notification into a non-local exit. An error code can then be produced at the target of this exit. You can thus write code like TRY_MSVC_INVAL { } CATCH_MSVC_INVAL { } DONE_MSVC_INVAL; This entire block expands to a single statement. The handling of invalid parameters can be done in three ways: * The default way, which is reasonable for programs (not libraries): AC_DEFINE([MSVC_INVALID_PARAMETER_HANDLING], [DEFAULT_HANDLING]) * The way for libraries that make "hairy" calls (like close(-1), or fclose(fp) where fileno(fp) is closed, or simply getdtablesize()): AC_DEFINE([MSVC_INVALID_PARAMETER_HANDLING], [HAIRY_LIBRARY_HANDLING]) * The way for libraries that make no "hairy" calls: AC_DEFINE([MSVC_INVALID_PARAMETER_HANDLING], [SANE_LIBRARY_HANDLING]) */ #define DEFAULT_HANDLING 0 #define HAIRY_LIBRARY_HANDLING 1 #define SANE_LIBRARY_HANDLING 2 #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && !(MSVC_INVALID_PARAMETER_HANDLING == SANE_LIBRARY_HANDLING) /* A native Windows platform with the "invalid parameter handler" concept, and either DEFAULT_HANDLING or HAIRY_LIBRARY_HANDLING. */ # if MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING /* Default handling. */ # ifdef __cplusplus extern "C" { # endif /* Ensure that the invalid parameter handler in installed that just returns. Because we assume no other part of the program installs a different invalid parameter handler, this solution is multithread-safe. */ extern void gl_msvc_inval_ensure_handler (void); # ifdef __cplusplus } # endif # define TRY_MSVC_INVAL \ do \ { \ gl_msvc_inval_ensure_handler (); \ if (1) # define CATCH_MSVC_INVAL \ else # define DONE_MSVC_INVAL \ } \ while (0) # else /* Handling for hairy libraries. */ # include /* Gnulib can define its own status codes, as described in the page "Raising Software Exceptions" on microsoft.com . Our status codes are composed of - 0xE0000000, mandatory for all user-defined status codes, - 0x474E550, a API identifier ("GNU"), - 0, 1, 2, ..., used to distinguish different status codes from the same API. */ # define STATUS_GNULIB_INVALID_PARAMETER (0xE0000000 + 0x474E550 + 0) # if defined _MSC_VER /* A compiler that supports __try/__except, as described in the page "try-except statement" on microsoft.com . With __try/__except, we can use the multithread-safe exception handling. */ # ifdef __cplusplus extern "C" { # endif /* Ensure that the invalid parameter handler in installed that raises a software exception with code STATUS_GNULIB_INVALID_PARAMETER. Because we assume no other part of the program installs a different invalid parameter handler, this solution is multithread-safe. */ extern void gl_msvc_inval_ensure_handler (void); # ifdef __cplusplus } # endif # define TRY_MSVC_INVAL \ do \ { \ gl_msvc_inval_ensure_handler (); \ __try # define CATCH_MSVC_INVAL \ __except (GetExceptionCode () == STATUS_GNULIB_INVALID_PARAMETER \ ? EXCEPTION_EXECUTE_HANDLER \ : EXCEPTION_CONTINUE_SEARCH) # define DONE_MSVC_INVAL \ } \ while (0) # else /* Any compiler. We can only use setjmp/longjmp. */ # include # ifdef __cplusplus extern "C" { # endif struct gl_msvc_inval_per_thread { /* The restart that will resume execution at the code between CATCH_MSVC_INVAL and DONE_MSVC_INVAL. It is enabled only between TRY_MSVC_INVAL and CATCH_MSVC_INVAL. */ jmp_buf restart; /* Tells whether the contents of restart is valid. */ int restart_valid; }; /* Ensure that the invalid parameter handler in installed that passes control to the gl_msvc_inval_restart if it is valid, or raises a software exception with code STATUS_GNULIB_INVALID_PARAMETER otherwise. Because we assume no other part of the program installs a different invalid parameter handler, this solution is multithread-safe. */ extern void gl_msvc_inval_ensure_handler (void); /* Return a pointer to the per-thread data for the current thread. */ extern struct gl_msvc_inval_per_thread *gl_msvc_inval_current (void); # ifdef __cplusplus } # endif # define TRY_MSVC_INVAL \ do \ { \ struct gl_msvc_inval_per_thread *msvc_inval_current; \ gl_msvc_inval_ensure_handler (); \ msvc_inval_current = gl_msvc_inval_current (); \ /* First, initialize gl_msvc_inval_restart. */ \ if (setjmp (msvc_inval_current->restart) == 0) \ { \ /* Then, mark it as valid. */ \ msvc_inval_current->restart_valid = 1; # define CATCH_MSVC_INVAL \ /* Execution completed. \ Mark gl_msvc_inval_restart as invalid. */ \ msvc_inval_current->restart_valid = 0; \ } \ else \ { \ /* Execution triggered an invalid parameter notification. \ Mark gl_msvc_inval_restart as invalid. */ \ msvc_inval_current->restart_valid = 0; # define DONE_MSVC_INVAL \ } \ } \ while (0) # endif # endif #else /* A platform that does not need to the invalid parameter handler, or when SANE_LIBRARY_HANDLING is desired. */ /* The braces here avoid GCC warnings like "warning: suggest explicit braces to avoid ambiguous 'else'". */ # define TRY_MSVC_INVAL \ do \ { \ if (1) # define CATCH_MSVC_INVAL \ else # define DONE_MSVC_INVAL \ } \ while (0) #endif #endif /* _MSVC_INVAL_H */ gnuastro-0.5/bootstrapped/lib/memchr.valgrind0000644000175000017500000000065213217200021016407 00000000000000# Suppress a valgrind message about use of uninitialized memory in memchr(). # POSIX states that when the character is found, memchr must not read extra # bytes in an overestimated length (for example, where memchr is used to # implement strnlen). However, we use a safe word read to provide a speedup. { memchr-value4 Memcheck:Value4 fun:rpl_memchr } { memchr-value8 Memcheck:Value8 fun:rpl_memchr } gnuastro-0.5/bootstrapped/lib/mbtowc-impl.h0000644000175000017500000000262713217200021016013 00000000000000/* Convert multibyte character to wide character. Copyright (C) 2011-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* We don't need a static internal state, because the encoding is not state dependent, and when mbrtowc returns (size_t)(-2). we throw the result away. */ int mbtowc (wchar_t *pwc, const char *s, size_t n) { if (s == NULL) return 0; else { mbstate_t state; wchar_t wc; size_t result; memset (&state, 0, sizeof (mbstate_t)); result = mbrtowc (&wc, s, n, &state); if (result == (size_t)-1 || result == (size_t)-2) { errno = EILSEQ; return -1; } if (pwc != NULL) *pwc = wc; return (wc == 0 ? 0 : result); } } gnuastro-0.5/bootstrapped/lib/mbchar.h0000644000175000017500000003342513217200021015015 00000000000000/* Multibyte character data type. Copyright (C) 2001, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible . */ /* A multibyte character is a short subsequence of a char* string, representing a single wide character. We use multibyte characters instead of wide characters because of the following goals: 1) correct multibyte handling, i.e. operate according to the LC_CTYPE locale, 2) ease of maintenance, i.e. the maintainer needs not know all details of the ISO C 99 standard, 3) don't fail grossly if the input is not in the encoding set by the locale, because often different encodings are in use in the same countries (ISO-8859-1/UTF-8, EUC-JP/Shift_JIS, ...), 4) fast in the case of ASCII characters, 5) portability, i.e. don't make unportable assumptions about wchar_t. Multibyte characters are only accessed through the mb* macros. mb_ptr (mbc) return a pointer to the beginning of the multibyte sequence. mb_len (mbc) returns the number of bytes occupied by the multibyte sequence. Always > 0. mb_iseq (mbc, sc) returns true if mbc is the standard ASCII character sc. mb_isnul (mbc) returns true if mbc is the nul character. mb_cmp (mbc1, mbc2) returns a positive, zero, or negative value depending on whether mbc1 sorts after, same or before mbc2. mb_casecmp (mbc1, mbc2) returns a positive, zero, or negative value depending on whether mbc1 sorts after, same or before mbc2, modulo upper/lowercase conversion. mb_equal (mbc1, mbc2) returns true if mbc1 and mbc2 are equal. mb_caseequal (mbc1, mbc2) returns true if mbc1 and mbc2 are equal modulo upper/lowercase conversion. mb_isalnum (mbc) returns true if mbc is alphanumeric. mb_isalpha (mbc) returns true if mbc is alphabetic. mb_isascii(mbc) returns true if mbc is plain ASCII. mb_isblank (mbc) returns true if mbc is a blank. mb_iscntrl (mbc) returns true if mbc is a control character. mb_isdigit (mbc) returns true if mbc is a decimal digit. mb_isgraph (mbc) returns true if mbc is a graphic character. mb_islower (mbc) returns true if mbc is lowercase. mb_isprint (mbc) returns true if mbc is a printable character. mb_ispunct (mbc) returns true if mbc is a punctuation character. mb_isspace (mbc) returns true if mbc is a space character. mb_isupper (mbc) returns true if mbc is uppercase. mb_isxdigit (mbc) returns true if mbc is a hexadecimal digit. mb_width (mbc) returns the number of columns on the output device occupied by mbc. Always >= 0. mb_putc (mbc, stream) outputs mbc on stream, a byte oriented FILE stream opened for output. mb_setascii (&mbc, sc) assigns the standard ASCII character sc to mbc. mb_copy (&destmbc, &srcmbc) copies srcmbc to destmbc. Here are the function prototypes of the macros. extern const char * mb_ptr (const mbchar_t mbc); extern size_t mb_len (const mbchar_t mbc); extern bool mb_iseq (const mbchar_t mbc, char sc); extern bool mb_isnul (const mbchar_t mbc); extern int mb_cmp (const mbchar_t mbc1, const mbchar_t mbc2); extern int mb_casecmp (const mbchar_t mbc1, const mbchar_t mbc2); extern bool mb_equal (const mbchar_t mbc1, const mbchar_t mbc2); extern bool mb_caseequal (const mbchar_t mbc1, const mbchar_t mbc2); extern bool mb_isalnum (const mbchar_t mbc); extern bool mb_isalpha (const mbchar_t mbc); extern bool mb_isascii (const mbchar_t mbc); extern bool mb_isblank (const mbchar_t mbc); extern bool mb_iscntrl (const mbchar_t mbc); extern bool mb_isdigit (const mbchar_t mbc); extern bool mb_isgraph (const mbchar_t mbc); extern bool mb_islower (const mbchar_t mbc); extern bool mb_isprint (const mbchar_t mbc); extern bool mb_ispunct (const mbchar_t mbc); extern bool mb_isspace (const mbchar_t mbc); extern bool mb_isupper (const mbchar_t mbc); extern bool mb_isxdigit (const mbchar_t mbc); extern int mb_width (const mbchar_t mbc); extern void mb_putc (const mbchar_t mbc, FILE *stream); extern void mb_setascii (mbchar_t *new, char sc); extern void mb_copy (mbchar_t *new, const mbchar_t *old); */ #ifndef _MBCHAR_H #define _MBCHAR_H 1 #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.1 has a bug: and must be included before . */ #include #include #include #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef MBCHAR_INLINE # define MBCHAR_INLINE _GL_INLINE #endif #define MBCHAR_BUF_SIZE 24 struct mbchar { const char *ptr; /* pointer to current character */ size_t bytes; /* number of bytes of current character, > 0 */ bool wc_valid; /* true if wc is a valid wide character */ wchar_t wc; /* if wc_valid: the current character */ char buf[MBCHAR_BUF_SIZE]; /* room for the bytes, used for file input only */ }; /* EOF (not a real character) is represented with bytes = 0 and wc_valid = false. */ typedef struct mbchar mbchar_t; /* Access the current character. */ #define mb_ptr(mbc) ((mbc).ptr) #define mb_len(mbc) ((mbc).bytes) /* Comparison of characters. */ #define mb_iseq(mbc, sc) ((mbc).wc_valid && (mbc).wc == (sc)) #define mb_isnul(mbc) ((mbc).wc_valid && (mbc).wc == 0) #define mb_cmp(mbc1, mbc2) \ ((mbc1).wc_valid \ ? ((mbc2).wc_valid \ ? (int) (mbc1).wc - (int) (mbc2).wc \ : -1) \ : ((mbc2).wc_valid \ ? 1 \ : (mbc1).bytes == (mbc2).bytes \ ? memcmp ((mbc1).ptr, (mbc2).ptr, (mbc1).bytes) \ : (mbc1).bytes < (mbc2).bytes \ ? (memcmp ((mbc1).ptr, (mbc2).ptr, (mbc1).bytes) > 0 ? 1 : -1) \ : (memcmp ((mbc1).ptr, (mbc2).ptr, (mbc2).bytes) >= 0 ? 1 : -1))) #define mb_casecmp(mbc1, mbc2) \ ((mbc1).wc_valid \ ? ((mbc2).wc_valid \ ? (int) towlower ((mbc1).wc) - (int) towlower ((mbc2).wc) \ : -1) \ : ((mbc2).wc_valid \ ? 1 \ : (mbc1).bytes == (mbc2).bytes \ ? memcmp ((mbc1).ptr, (mbc2).ptr, (mbc1).bytes) \ : (mbc1).bytes < (mbc2).bytes \ ? (memcmp ((mbc1).ptr, (mbc2).ptr, (mbc1).bytes) > 0 ? 1 : -1) \ : (memcmp ((mbc1).ptr, (mbc2).ptr, (mbc2).bytes) >= 0 ? 1 : -1))) #define mb_equal(mbc1, mbc2) \ ((mbc1).wc_valid && (mbc2).wc_valid \ ? (mbc1).wc == (mbc2).wc \ : (mbc1).bytes == (mbc2).bytes \ && memcmp ((mbc1).ptr, (mbc2).ptr, (mbc1).bytes) == 0) #define mb_caseequal(mbc1, mbc2) \ ((mbc1).wc_valid && (mbc2).wc_valid \ ? towlower ((mbc1).wc) == towlower ((mbc2).wc) \ : (mbc1).bytes == (mbc2).bytes \ && memcmp ((mbc1).ptr, (mbc2).ptr, (mbc1).bytes) == 0) /* , classification. */ #define mb_isascii(mbc) \ ((mbc).wc_valid && (mbc).wc >= 0 && (mbc).wc <= 127) #define mb_isalnum(mbc) ((mbc).wc_valid && iswalnum ((mbc).wc)) #define mb_isalpha(mbc) ((mbc).wc_valid && iswalpha ((mbc).wc)) #define mb_isblank(mbc) ((mbc).wc_valid && iswblank ((mbc).wc)) #define mb_iscntrl(mbc) ((mbc).wc_valid && iswcntrl ((mbc).wc)) #define mb_isdigit(mbc) ((mbc).wc_valid && iswdigit ((mbc).wc)) #define mb_isgraph(mbc) ((mbc).wc_valid && iswgraph ((mbc).wc)) #define mb_islower(mbc) ((mbc).wc_valid && iswlower ((mbc).wc)) #define mb_isprint(mbc) ((mbc).wc_valid && iswprint ((mbc).wc)) #define mb_ispunct(mbc) ((mbc).wc_valid && iswpunct ((mbc).wc)) #define mb_isspace(mbc) ((mbc).wc_valid && iswspace ((mbc).wc)) #define mb_isupper(mbc) ((mbc).wc_valid && iswupper ((mbc).wc)) #define mb_isxdigit(mbc) ((mbc).wc_valid && iswxdigit ((mbc).wc)) /* Extra function. */ /* Unprintable characters appear as a small box of width 1. */ #define MB_UNPRINTABLE_WIDTH 1 MBCHAR_INLINE int mb_width_aux (wint_t wc) { int w = wcwidth (wc); /* For unprintable characters, arbitrarily return 0 for control characters and MB_UNPRINTABLE_WIDTH otherwise. */ return (w >= 0 ? w : iswcntrl (wc) ? 0 : MB_UNPRINTABLE_WIDTH); } #define mb_width(mbc) \ ((mbc).wc_valid ? mb_width_aux ((mbc).wc) : MB_UNPRINTABLE_WIDTH) /* Output. */ #define mb_putc(mbc, stream) fwrite ((mbc).ptr, 1, (mbc).bytes, (stream)) /* Assignment. */ #define mb_setascii(mbc, sc) \ ((mbc)->ptr = (mbc)->buf, (mbc)->bytes = 1, (mbc)->wc_valid = 1, \ (mbc)->wc = (mbc)->buf[0] = (sc)) /* Copying a character. */ MBCHAR_INLINE void mb_copy (mbchar_t *new_mbc, const mbchar_t *old_mbc) { if (old_mbc->ptr == &old_mbc->buf[0]) { memcpy (&new_mbc->buf[0], &old_mbc->buf[0], old_mbc->bytes); new_mbc->ptr = &new_mbc->buf[0]; } else new_mbc->ptr = old_mbc->ptr; new_mbc->bytes = old_mbc->bytes; if ((new_mbc->wc_valid = old_mbc->wc_valid)) new_mbc->wc = old_mbc->wc; } /* is_basic(c) tests whether the single-byte character c is in the ISO C "basic character set". This is a convenience function, and is in this file only to share code between mbiter_multi.h and mbfile_multi.h. */ #if (' ' == 32) && ('!' == 33) && ('"' == 34) && ('#' == 35) \ && ('%' == 37) && ('&' == 38) && ('\'' == 39) && ('(' == 40) \ && (')' == 41) && ('*' == 42) && ('+' == 43) && (',' == 44) \ && ('-' == 45) && ('.' == 46) && ('/' == 47) && ('0' == 48) \ && ('1' == 49) && ('2' == 50) && ('3' == 51) && ('4' == 52) \ && ('5' == 53) && ('6' == 54) && ('7' == 55) && ('8' == 56) \ && ('9' == 57) && (':' == 58) && (';' == 59) && ('<' == 60) \ && ('=' == 61) && ('>' == 62) && ('?' == 63) && ('A' == 65) \ && ('B' == 66) && ('C' == 67) && ('D' == 68) && ('E' == 69) \ && ('F' == 70) && ('G' == 71) && ('H' == 72) && ('I' == 73) \ && ('J' == 74) && ('K' == 75) && ('L' == 76) && ('M' == 77) \ && ('N' == 78) && ('O' == 79) && ('P' == 80) && ('Q' == 81) \ && ('R' == 82) && ('S' == 83) && ('T' == 84) && ('U' == 85) \ && ('V' == 86) && ('W' == 87) && ('X' == 88) && ('Y' == 89) \ && ('Z' == 90) && ('[' == 91) && ('\\' == 92) && (']' == 93) \ && ('^' == 94) && ('_' == 95) && ('a' == 97) && ('b' == 98) \ && ('c' == 99) && ('d' == 100) && ('e' == 101) && ('f' == 102) \ && ('g' == 103) && ('h' == 104) && ('i' == 105) && ('j' == 106) \ && ('k' == 107) && ('l' == 108) && ('m' == 109) && ('n' == 110) \ && ('o' == 111) && ('p' == 112) && ('q' == 113) && ('r' == 114) \ && ('s' == 115) && ('t' == 116) && ('u' == 117) && ('v' == 118) \ && ('w' == 119) && ('x' == 120) && ('y' == 121) && ('z' == 122) \ && ('{' == 123) && ('|' == 124) && ('}' == 125) && ('~' == 126) /* The character set is ISO-646, not EBCDIC. */ # define IS_BASIC_ASCII 1 extern const unsigned int is_basic_table[]; MBCHAR_INLINE bool is_basic (char c) { return (is_basic_table [(unsigned char) c >> 5] >> ((unsigned char) c & 31)) & 1; } #else MBCHAR_INLINE bool is_basic (char c) { switch (c) { case '\t': case '\v': case '\f': case ' ': case '!': case '"': case '#': case '%': case '&': case '\'': case '(': case ')': case '*': case '+': case ',': case '-': case '.': case '/': case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': case ':': case ';': case '<': case '=': case '>': case '?': case 'A': case 'B': case 'C': case 'D': case 'E': case 'F': case 'G': case 'H': case 'I': case 'J': case 'K': case 'L': case 'M': case 'N': case 'O': case 'P': case 'Q': case 'R': case 'S': case 'T': case 'U': case 'V': case 'W': case 'X': case 'Y': case 'Z': case '[': case '\\': case ']': case '^': case '_': case 'a': case 'b': case 'c': case 'd': case 'e': case 'f': case 'g': case 'h': case 'i': case 'j': case 'k': case 'l': case 'm': case 'n': case 'o': case 'p': case 'q': case 'r': case 's': case 't': case 'u': case 'v': case 'w': case 'x': case 'y': case 'z': case '{': case '|': case '}': case '~': return 1; default: return 0; } } #endif _GL_INLINE_HEADER_END #endif /* _MBCHAR_H */ gnuastro-0.5/bootstrapped/lib/math.in.h0000644000175000017500000020755413217200021015125 00000000000000/* A GNU-like . Copyright (C) 2002-2003, 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _@GUARD_PREFIX@_MATH_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ #ifndef _@GUARD_PREFIX@_MATH_H #define _@GUARD_PREFIX@_MATH_H /* On OpenVMS, NAN, INFINITY, and HUGEVAL macros are defined in . */ #if defined __VMS && ! defined NAN # include #endif #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef _GL_MATH_INLINE # define _GL_MATH_INLINE _GL_INLINE #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ #ifdef __cplusplus /* Helper macros to define type-generic function FUNC as overloaded functions, rather than as macros like in C. POSIX declares these with an argument of real-floating (that is, one of float, double, or long double). */ # define _GL_MATH_CXX_REAL_FLOATING_DECL_1(func) \ static inline int \ _gl_cxx_ ## func ## f (float f) \ { \ return func (f); \ } \ static inline int \ _gl_cxx_ ## func ## d (double d) \ { \ return func (d); \ } \ static inline int \ _gl_cxx_ ## func ## l (long double l) \ { \ return func (l); \ } # define _GL_MATH_CXX_REAL_FLOATING_DECL_2(func) \ _GL_BEGIN_NAMESPACE \ inline int \ func (float f) \ { \ return _gl_cxx_ ## func ## f (f); \ } \ inline int \ func (double d) \ { \ return _gl_cxx_ ## func ## d (d); \ } \ inline int \ func (long double l) \ { \ return _gl_cxx_ ## func ## l (l); \ } \ _GL_END_NAMESPACE #endif /* Helper macros to define a portability warning for the classification macro FUNC called with VALUE. POSIX declares the classification macros with an argument of real-floating (that is, one of float, double, or long double). */ #define _GL_WARN_REAL_FLOATING_DECL(func) \ _GL_MATH_INLINE int \ rpl_ ## func ## f (float f) \ { \ return func (f); \ } \ _GL_MATH_INLINE int \ rpl_ ## func ## d (double d) \ { \ return func (d); \ } \ _GL_MATH_INLINE int \ rpl_ ## func ## l (long double l) \ { \ return func (l); \ } \ _GL_WARN_ON_USE (rpl_ ## func ## f, #func " is unportable - " \ "use gnulib module " #func " for portability"); \ _GL_WARN_ON_USE (rpl_ ## func ## d, #func " is unportable - " \ "use gnulib module " #func " for portability"); \ _GL_WARN_ON_USE (rpl_ ## func ## l, #func " is unportable - " \ "use gnulib module " #func " for portability") #define _GL_WARN_REAL_FLOATING_IMPL(func, value) \ (sizeof (value) == sizeof (float) ? rpl_ ## func ## f (value) \ : sizeof (value) == sizeof (double) ? rpl_ ## func ## d (value) \ : rpl_ ## func ## l (value)) #if @REPLACE_ITOLD@ /* Pull in a function that fixes the 'int' to 'long double' conversion of glibc 2.7. */ _GL_EXTERN_C void _Qp_itoq (long double *, int); static void (*_gl_math_fix_itold) (long double *, int) = _Qp_itoq; #endif /* POSIX allows platforms that don't support NAN. But all major machines in the past 15 years have supported something close to IEEE NaN, so we define this unconditionally. We also must define it on platforms like Solaris 10, where NAN is present but defined as a function pointer rather than a floating point constant. */ #if !defined NAN || @REPLACE_NAN@ # if !GNULIB_defined_NAN # undef NAN /* The Compaq (ex-DEC) C 6.4 compiler and the Microsoft MSVC 9 compiler choke on the expression 0.0 / 0.0. */ # if defined __DECC || defined _MSC_VER _GL_MATH_INLINE float _NaN () { static float zero = 0.0f; return zero / zero; } # define NAN (_NaN()) # else # define NAN (0.0f / 0.0f) # endif # define GNULIB_defined_NAN 1 # endif #endif /* Solaris 10 defines HUGE_VAL, but as a function pointer rather than a floating point constant. */ #if @REPLACE_HUGE_VAL@ # undef HUGE_VALF # define HUGE_VALF (1.0f / 0.0f) # undef HUGE_VAL # define HUGE_VAL (1.0 / 0.0) # undef HUGE_VALL # define HUGE_VALL (1.0L / 0.0L) #endif /* HUGE_VALF is a 'float' Infinity. */ #ifndef HUGE_VALF # if defined _MSC_VER /* The Microsoft MSVC 9 compiler chokes on the expression 1.0f / 0.0f. */ # define HUGE_VALF (1e25f * 1e25f) # else # define HUGE_VALF (1.0f / 0.0f) # endif #endif /* HUGE_VAL is a 'double' Infinity. */ #ifndef HUGE_VAL # if defined _MSC_VER /* The Microsoft MSVC 9 compiler chokes on the expression 1.0 / 0.0. */ # define HUGE_VAL (1e250 * 1e250) # else # define HUGE_VAL (1.0 / 0.0) # endif #endif /* HUGE_VALL is a 'long double' Infinity. */ #ifndef HUGE_VALL # if defined _MSC_VER /* The Microsoft MSVC 9 compiler chokes on the expression 1.0L / 0.0L. */ # define HUGE_VALL (1e250L * 1e250L) # else # define HUGE_VALL (1.0L / 0.0L) # endif #endif #if defined FP_ILOGB0 && defined FP_ILOGBNAN /* Ensure FP_ILOGB0 and FP_ILOGBNAN are correct. */ # if defined __HAIKU__ /* Haiku: match what ilogb() does */ # undef FP_ILOGB0 # undef FP_ILOGBNAN # define FP_ILOGB0 (- 2147483647 - 1) /* INT_MIN */ # define FP_ILOGBNAN (- 2147483647 - 1) /* INT_MIN */ # endif #else /* Ensure FP_ILOGB0 and FP_ILOGBNAN are defined. */ # if defined __NetBSD__ || defined __sgi /* NetBSD, IRIX 6.5: match what ilogb() does */ # define FP_ILOGB0 (- 2147483647 - 1) /* INT_MIN */ # define FP_ILOGBNAN (- 2147483647 - 1) /* INT_MIN */ # elif defined _AIX /* AIX 5.1: match what ilogb() does in AIX >= 5.2 */ # define FP_ILOGB0 (- 2147483647 - 1) /* INT_MIN */ # define FP_ILOGBNAN 2147483647 /* INT_MAX */ # elif defined __sun /* Solaris 9: match what ilogb() does */ # define FP_ILOGB0 (- 2147483647) /* - INT_MAX */ # define FP_ILOGBNAN 2147483647 /* INT_MAX */ # else /* Gnulib defined values. */ # define FP_ILOGB0 (- 2147483647) /* - INT_MAX */ # define FP_ILOGBNAN (- 2147483647 - 1) /* INT_MIN */ # endif #endif #if @GNULIB_ACOSF@ # if @REPLACE_ACOSF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef acosf # define acosf rpl_acosf # endif _GL_FUNCDECL_RPL (acosf, float, (float x)); _GL_CXXALIAS_RPL (acosf, float, (float x)); # else # if !@HAVE_ACOSF@ # undef acosf _GL_FUNCDECL_SYS (acosf, float, (float x)); # endif _GL_CXXALIAS_SYS (acosf, float, (float x)); # endif _GL_CXXALIASWARN (acosf); #elif defined GNULIB_POSIXCHECK # undef acosf # if HAVE_RAW_DECL_ACOSF _GL_WARN_ON_USE (acosf, "acosf is unportable - " "use gnulib module acosf for portability"); # endif #endif #if @GNULIB_ACOSL@ # if !@HAVE_ACOSL@ || !@HAVE_DECL_ACOSL@ # undef acosl _GL_FUNCDECL_SYS (acosl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (acosl, long double, (long double x)); _GL_CXXALIASWARN (acosl); #elif defined GNULIB_POSIXCHECK # undef acosl # if HAVE_RAW_DECL_ACOSL _GL_WARN_ON_USE (acosl, "acosl is unportable - " "use gnulib module acosl for portability"); # endif #endif #if @GNULIB_ASINF@ # if @REPLACE_ASINF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef asinf # define asinf rpl_asinf # endif _GL_FUNCDECL_RPL (asinf, float, (float x)); _GL_CXXALIAS_RPL (asinf, float, (float x)); # else # if !@HAVE_ASINF@ # undef asinf _GL_FUNCDECL_SYS (asinf, float, (float x)); # endif _GL_CXXALIAS_SYS (asinf, float, (float x)); # endif _GL_CXXALIASWARN (asinf); #elif defined GNULIB_POSIXCHECK # undef asinf # if HAVE_RAW_DECL_ASINF _GL_WARN_ON_USE (asinf, "asinf is unportable - " "use gnulib module asinf for portability"); # endif #endif #if @GNULIB_ASINL@ # if !@HAVE_ASINL@ || !@HAVE_DECL_ASINL@ # undef asinl _GL_FUNCDECL_SYS (asinl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (asinl, long double, (long double x)); _GL_CXXALIASWARN (asinl); #elif defined GNULIB_POSIXCHECK # undef asinl # if HAVE_RAW_DECL_ASINL _GL_WARN_ON_USE (asinl, "asinl is unportable - " "use gnulib module asinl for portability"); # endif #endif #if @GNULIB_ATANF@ # if @REPLACE_ATANF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef atanf # define atanf rpl_atanf # endif _GL_FUNCDECL_RPL (atanf, float, (float x)); _GL_CXXALIAS_RPL (atanf, float, (float x)); # else # if !@HAVE_ATANF@ # undef atanf _GL_FUNCDECL_SYS (atanf, float, (float x)); # endif _GL_CXXALIAS_SYS (atanf, float, (float x)); # endif _GL_CXXALIASWARN (atanf); #elif defined GNULIB_POSIXCHECK # undef atanf # if HAVE_RAW_DECL_ATANF _GL_WARN_ON_USE (atanf, "atanf is unportable - " "use gnulib module atanf for portability"); # endif #endif #if @GNULIB_ATANL@ # if !@HAVE_ATANL@ || !@HAVE_DECL_ATANL@ # undef atanl _GL_FUNCDECL_SYS (atanl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (atanl, long double, (long double x)); _GL_CXXALIASWARN (atanl); #elif defined GNULIB_POSIXCHECK # undef atanl # if HAVE_RAW_DECL_ATANL _GL_WARN_ON_USE (atanl, "atanl is unportable - " "use gnulib module atanl for portability"); # endif #endif #if @GNULIB_ATAN2F@ # if @REPLACE_ATAN2F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef atan2f # define atan2f rpl_atan2f # endif _GL_FUNCDECL_RPL (atan2f, float, (float y, float x)); _GL_CXXALIAS_RPL (atan2f, float, (float y, float x)); # else # if !@HAVE_ATAN2F@ # undef atan2f _GL_FUNCDECL_SYS (atan2f, float, (float y, float x)); # endif _GL_CXXALIAS_SYS (atan2f, float, (float y, float x)); # endif _GL_CXXALIASWARN (atan2f); #elif defined GNULIB_POSIXCHECK # undef atan2f # if HAVE_RAW_DECL_ATAN2F _GL_WARN_ON_USE (atan2f, "atan2f is unportable - " "use gnulib module atan2f for portability"); # endif #endif #if @GNULIB_CBRTF@ # if @REPLACE_CBRTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef cbrtf # define cbrtf rpl_cbrtf # endif _GL_FUNCDECL_RPL (cbrtf, float, (float x)); _GL_CXXALIAS_RPL (cbrtf, float, (float x)); # else # if !@HAVE_DECL_CBRTF@ _GL_FUNCDECL_SYS (cbrtf, float, (float x)); # endif _GL_CXXALIAS_SYS (cbrtf, float, (float x)); # endif _GL_CXXALIASWARN (cbrtf); #elif defined GNULIB_POSIXCHECK # undef cbrtf # if HAVE_RAW_DECL_CBRTF _GL_WARN_ON_USE (cbrtf, "cbrtf is unportable - " "use gnulib module cbrtf for portability"); # endif #endif #if @GNULIB_CBRT@ # if !@HAVE_CBRT@ _GL_FUNCDECL_SYS (cbrt, double, (double x)); # endif _GL_CXXALIAS_SYS (cbrt, double, (double x)); _GL_CXXALIASWARN (cbrt); #elif defined GNULIB_POSIXCHECK # undef cbrt # if HAVE_RAW_DECL_CBRT _GL_WARN_ON_USE (cbrt, "cbrt is unportable - " "use gnulib module cbrt for portability"); # endif #endif #if @GNULIB_CBRTL@ # if @REPLACE_CBRTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef cbrtl # define cbrtl rpl_cbrtl # endif _GL_FUNCDECL_RPL (cbrtl, long double, (long double x)); _GL_CXXALIAS_RPL (cbrtl, long double, (long double x)); # else # if !@HAVE_DECL_CBRTL@ _GL_FUNCDECL_SYS (cbrtl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (cbrtl, long double, (long double x)); # endif _GL_CXXALIASWARN (cbrtl); #elif defined GNULIB_POSIXCHECK # undef cbrtl # if HAVE_RAW_DECL_CBRTL _GL_WARN_ON_USE (cbrtl, "cbrtl is unportable - " "use gnulib module cbrtl for portability"); # endif #endif #if @GNULIB_CEILF@ # if @REPLACE_CEILF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ceilf # define ceilf rpl_ceilf # endif _GL_FUNCDECL_RPL (ceilf, float, (float x)); _GL_CXXALIAS_RPL (ceilf, float, (float x)); # else # if !@HAVE_DECL_CEILF@ # undef ceilf _GL_FUNCDECL_SYS (ceilf, float, (float x)); # endif _GL_CXXALIAS_SYS (ceilf, float, (float x)); # endif _GL_CXXALIASWARN (ceilf); #elif defined GNULIB_POSIXCHECK # undef ceilf # if HAVE_RAW_DECL_CEILF _GL_WARN_ON_USE (ceilf, "ceilf is unportable - " "use gnulib module ceilf for portability"); # endif #endif #if @GNULIB_CEIL@ # if @REPLACE_CEIL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ceil # define ceil rpl_ceil # endif _GL_FUNCDECL_RPL (ceil, double, (double x)); _GL_CXXALIAS_RPL (ceil, double, (double x)); # else _GL_CXXALIAS_SYS (ceil, double, (double x)); # endif _GL_CXXALIASWARN (ceil); #endif #if @GNULIB_CEILL@ # if @REPLACE_CEILL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ceill # define ceill rpl_ceill # endif _GL_FUNCDECL_RPL (ceill, long double, (long double x)); _GL_CXXALIAS_RPL (ceill, long double, (long double x)); # else # if !@HAVE_DECL_CEILL@ # undef ceill _GL_FUNCDECL_SYS (ceill, long double, (long double x)); # endif _GL_CXXALIAS_SYS (ceill, long double, (long double x)); # endif _GL_CXXALIASWARN (ceill); #elif defined GNULIB_POSIXCHECK # undef ceill # if HAVE_RAW_DECL_CEILL _GL_WARN_ON_USE (ceill, "ceill is unportable - " "use gnulib module ceill for portability"); # endif #endif #if @GNULIB_COPYSIGNF@ # if !@HAVE_DECL_COPYSIGNF@ _GL_FUNCDECL_SYS (copysignf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (copysignf, float, (float x, float y)); _GL_CXXALIASWARN (copysignf); #elif defined GNULIB_POSIXCHECK # undef copysignf # if HAVE_RAW_DECL_COPYSIGNF _GL_WARN_ON_USE (copysignf, "copysignf is unportable - " "use gnulib module copysignf for portability"); # endif #endif #if @GNULIB_COPYSIGN@ # if !@HAVE_COPYSIGN@ _GL_FUNCDECL_SYS (copysign, double, (double x, double y)); # endif _GL_CXXALIAS_SYS (copysign, double, (double x, double y)); _GL_CXXALIASWARN (copysign); #elif defined GNULIB_POSIXCHECK # undef copysign # if HAVE_RAW_DECL_COPYSIGN _GL_WARN_ON_USE (copysign, "copysign is unportable - " "use gnulib module copysign for portability"); # endif #endif #if @GNULIB_COPYSIGNL@ # if !@HAVE_COPYSIGNL@ _GL_FUNCDECL_SYS (copysignl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (copysignl, long double, (long double x, long double y)); _GL_CXXALIASWARN (copysignl); #elif defined GNULIB_POSIXCHECK # undef copysignl # if HAVE_RAW_DECL_COPYSIGNL _GL_WARN_ON_USE (copysign, "copysignl is unportable - " "use gnulib module copysignl for portability"); # endif #endif #if @GNULIB_COSF@ # if @REPLACE_COSF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef cosf # define cosf rpl_cosf # endif _GL_FUNCDECL_RPL (cosf, float, (float x)); _GL_CXXALIAS_RPL (cosf, float, (float x)); # else # if !@HAVE_COSF@ # undef cosf _GL_FUNCDECL_SYS (cosf, float, (float x)); # endif _GL_CXXALIAS_SYS (cosf, float, (float x)); # endif _GL_CXXALIASWARN (cosf); #elif defined GNULIB_POSIXCHECK # undef cosf # if HAVE_RAW_DECL_COSF _GL_WARN_ON_USE (cosf, "cosf is unportable - " "use gnulib module cosf for portability"); # endif #endif #if @GNULIB_COSL@ # if !@HAVE_COSL@ || !@HAVE_DECL_COSL@ # undef cosl _GL_FUNCDECL_SYS (cosl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (cosl, long double, (long double x)); _GL_CXXALIASWARN (cosl); #elif defined GNULIB_POSIXCHECK # undef cosl # if HAVE_RAW_DECL_COSL _GL_WARN_ON_USE (cosl, "cosl is unportable - " "use gnulib module cosl for portability"); # endif #endif #if @GNULIB_COSHF@ # if @REPLACE_COSHF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef coshf # define coshf rpl_coshf # endif _GL_FUNCDECL_RPL (coshf, float, (float x)); _GL_CXXALIAS_RPL (coshf, float, (float x)); # else # if !@HAVE_COSHF@ # undef coshf _GL_FUNCDECL_SYS (coshf, float, (float x)); # endif _GL_CXXALIAS_SYS (coshf, float, (float x)); # endif _GL_CXXALIASWARN (coshf); #elif defined GNULIB_POSIXCHECK # undef coshf # if HAVE_RAW_DECL_COSHF _GL_WARN_ON_USE (coshf, "coshf is unportable - " "use gnulib module coshf for portability"); # endif #endif #if @GNULIB_EXPF@ # if @REPLACE_EXPF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef expf # define expf rpl_expf # endif _GL_FUNCDECL_RPL (expf, float, (float x)); _GL_CXXALIAS_RPL (expf, float, (float x)); # else # if !@HAVE_EXPF@ # undef expf _GL_FUNCDECL_SYS (expf, float, (float x)); # endif _GL_CXXALIAS_SYS (expf, float, (float x)); # endif _GL_CXXALIASWARN (expf); #elif defined GNULIB_POSIXCHECK # undef expf # if HAVE_RAW_DECL_EXPF _GL_WARN_ON_USE (expf, "expf is unportable - " "use gnulib module expf for portability"); # endif #endif #if @GNULIB_EXPL@ # if !@HAVE_EXPL@ || !@HAVE_DECL_EXPL@ # undef expl _GL_FUNCDECL_SYS (expl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (expl, long double, (long double x)); _GL_CXXALIASWARN (expl); #elif defined GNULIB_POSIXCHECK # undef expl # if HAVE_RAW_DECL_EXPL _GL_WARN_ON_USE (expl, "expl is unportable - " "use gnulib module expl for portability"); # endif #endif #if @GNULIB_EXP2F@ # if !@HAVE_DECL_EXP2F@ _GL_FUNCDECL_SYS (exp2f, float, (float x)); # endif _GL_CXXALIAS_SYS (exp2f, float, (float x)); _GL_CXXALIASWARN (exp2f); #elif defined GNULIB_POSIXCHECK # undef exp2f # if HAVE_RAW_DECL_EXP2F _GL_WARN_ON_USE (exp2f, "exp2f is unportable - " "use gnulib module exp2f for portability"); # endif #endif #if @GNULIB_EXP2@ # if @REPLACE_EXP2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef exp2 # define exp2 rpl_exp2 # endif _GL_FUNCDECL_RPL (exp2, double, (double x)); _GL_CXXALIAS_RPL (exp2, double, (double x)); # else # if !@HAVE_DECL_EXP2@ _GL_FUNCDECL_SYS (exp2, double, (double x)); # endif _GL_CXXALIAS_SYS (exp2, double, (double x)); # endif _GL_CXXALIASWARN (exp2); #elif defined GNULIB_POSIXCHECK # undef exp2 # if HAVE_RAW_DECL_EXP2 _GL_WARN_ON_USE (exp2, "exp2 is unportable - " "use gnulib module exp2 for portability"); # endif #endif #if @GNULIB_EXP2L@ # if @REPLACE_EXP2L@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef exp2l # define exp2l rpl_exp2l # endif _GL_FUNCDECL_RPL (exp2l, long double, (long double x)); _GL_CXXALIAS_RPL (exp2l, long double, (long double x)); # else # if !@HAVE_DECL_EXP2L@ # undef exp2l _GL_FUNCDECL_SYS (exp2l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (exp2l, long double, (long double x)); # endif _GL_CXXALIASWARN (exp2l); #elif defined GNULIB_POSIXCHECK # undef exp2l # if HAVE_RAW_DECL_EXP2L _GL_WARN_ON_USE (exp2l, "exp2l is unportable - " "use gnulib module exp2l for portability"); # endif #endif #if @GNULIB_EXPM1F@ # if @REPLACE_EXPM1F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef expm1f # define expm1f rpl_expm1f # endif _GL_FUNCDECL_RPL (expm1f, float, (float x)); _GL_CXXALIAS_RPL (expm1f, float, (float x)); # else # if !@HAVE_EXPM1F@ _GL_FUNCDECL_SYS (expm1f, float, (float x)); # endif _GL_CXXALIAS_SYS (expm1f, float, (float x)); # endif _GL_CXXALIASWARN (expm1f); #elif defined GNULIB_POSIXCHECK # undef expm1f # if HAVE_RAW_DECL_EXPM1F _GL_WARN_ON_USE (expm1f, "expm1f is unportable - " "use gnulib module expm1f for portability"); # endif #endif #if @GNULIB_EXPM1@ # if @REPLACE_EXPM1@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef expm1 # define expm1 rpl_expm1 # endif _GL_FUNCDECL_RPL (expm1, double, (double x)); _GL_CXXALIAS_RPL (expm1, double, (double x)); # else # if !@HAVE_EXPM1@ _GL_FUNCDECL_SYS (expm1, double, (double x)); # endif _GL_CXXALIAS_SYS (expm1, double, (double x)); # endif _GL_CXXALIASWARN (expm1); #elif defined GNULIB_POSIXCHECK # undef expm1 # if HAVE_RAW_DECL_EXPM1 _GL_WARN_ON_USE (expm1, "expm1 is unportable - " "use gnulib module expm1 for portability"); # endif #endif #if @GNULIB_EXPM1L@ # if !@HAVE_DECL_EXPM1L@ # undef expm1l _GL_FUNCDECL_SYS (expm1l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (expm1l, long double, (long double x)); _GL_CXXALIASWARN (expm1l); #elif defined GNULIB_POSIXCHECK # undef expm1l # if HAVE_RAW_DECL_EXPM1L _GL_WARN_ON_USE (expm1l, "expm1l is unportable - " "use gnulib module expm1l for portability"); # endif #endif #if @GNULIB_FABSF@ # if !@HAVE_FABSF@ # undef fabsf _GL_FUNCDECL_SYS (fabsf, float, (float x)); # endif _GL_CXXALIAS_SYS (fabsf, float, (float x)); _GL_CXXALIASWARN (fabsf); #elif defined GNULIB_POSIXCHECK # undef fabsf # if HAVE_RAW_DECL_FABSF _GL_WARN_ON_USE (fabsf, "fabsf is unportable - " "use gnulib module fabsf for portability"); # endif #endif #if @GNULIB_FABSL@ # if @REPLACE_FABSL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fabsl # define fabsl rpl_fabsl # endif _GL_FUNCDECL_RPL (fabsl, long double, (long double x)); _GL_CXXALIAS_RPL (fabsl, long double, (long double x)); # else # if !@HAVE_FABSL@ # undef fabsl _GL_FUNCDECL_SYS (fabsl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (fabsl, long double, (long double x)); # endif _GL_CXXALIASWARN (fabsl); #elif defined GNULIB_POSIXCHECK # undef fabsl # if HAVE_RAW_DECL_FABSL _GL_WARN_ON_USE (fabsl, "fabsl is unportable - " "use gnulib module fabsl for portability"); # endif #endif #if @GNULIB_FLOORF@ # if @REPLACE_FLOORF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef floorf # define floorf rpl_floorf # endif _GL_FUNCDECL_RPL (floorf, float, (float x)); _GL_CXXALIAS_RPL (floorf, float, (float x)); # else # if !@HAVE_DECL_FLOORF@ # undef floorf _GL_FUNCDECL_SYS (floorf, float, (float x)); # endif _GL_CXXALIAS_SYS (floorf, float, (float x)); # endif _GL_CXXALIASWARN (floorf); #elif defined GNULIB_POSIXCHECK # undef floorf # if HAVE_RAW_DECL_FLOORF _GL_WARN_ON_USE (floorf, "floorf is unportable - " "use gnulib module floorf for portability"); # endif #endif #if @GNULIB_FLOOR@ # if @REPLACE_FLOOR@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef floor # define floor rpl_floor # endif _GL_FUNCDECL_RPL (floor, double, (double x)); _GL_CXXALIAS_RPL (floor, double, (double x)); # else _GL_CXXALIAS_SYS (floor, double, (double x)); # endif _GL_CXXALIASWARN (floor); #endif #if @GNULIB_FLOORL@ # if @REPLACE_FLOORL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef floorl # define floorl rpl_floorl # endif _GL_FUNCDECL_RPL (floorl, long double, (long double x)); _GL_CXXALIAS_RPL (floorl, long double, (long double x)); # else # if !@HAVE_DECL_FLOORL@ # undef floorl _GL_FUNCDECL_SYS (floorl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (floorl, long double, (long double x)); # endif _GL_CXXALIASWARN (floorl); #elif defined GNULIB_POSIXCHECK # undef floorl # if HAVE_RAW_DECL_FLOORL _GL_WARN_ON_USE (floorl, "floorl is unportable - " "use gnulib module floorl for portability"); # endif #endif #if @GNULIB_FMAF@ # if @REPLACE_FMAF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmaf # define fmaf rpl_fmaf # endif _GL_FUNCDECL_RPL (fmaf, float, (float x, float y, float z)); _GL_CXXALIAS_RPL (fmaf, float, (float x, float y, float z)); # else # if !@HAVE_FMAF@ _GL_FUNCDECL_SYS (fmaf, float, (float x, float y, float z)); # endif _GL_CXXALIAS_SYS (fmaf, float, (float x, float y, float z)); # endif _GL_CXXALIASWARN (fmaf); #elif defined GNULIB_POSIXCHECK # undef fmaf # if HAVE_RAW_DECL_FMAF _GL_WARN_ON_USE (fmaf, "fmaf is unportable - " "use gnulib module fmaf for portability"); # endif #endif #if @GNULIB_FMA@ # if @REPLACE_FMA@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fma # define fma rpl_fma # endif _GL_FUNCDECL_RPL (fma, double, (double x, double y, double z)); _GL_CXXALIAS_RPL (fma, double, (double x, double y, double z)); # else # if !@HAVE_FMA@ _GL_FUNCDECL_SYS (fma, double, (double x, double y, double z)); # endif _GL_CXXALIAS_SYS (fma, double, (double x, double y, double z)); # endif _GL_CXXALIASWARN (fma); #elif defined GNULIB_POSIXCHECK # undef fma # if HAVE_RAW_DECL_FMA _GL_WARN_ON_USE (fma, "fma is unportable - " "use gnulib module fma for portability"); # endif #endif #if @GNULIB_FMAL@ # if @REPLACE_FMAL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmal # define fmal rpl_fmal # endif _GL_FUNCDECL_RPL (fmal, long double, (long double x, long double y, long double z)); _GL_CXXALIAS_RPL (fmal, long double, (long double x, long double y, long double z)); # else # if !@HAVE_FMAL@ # undef fmal _GL_FUNCDECL_SYS (fmal, long double, (long double x, long double y, long double z)); # endif _GL_CXXALIAS_SYS (fmal, long double, (long double x, long double y, long double z)); # endif _GL_CXXALIASWARN (fmal); #elif defined GNULIB_POSIXCHECK # undef fmal # if HAVE_RAW_DECL_FMAL _GL_WARN_ON_USE (fmal, "fmal is unportable - " "use gnulib module fmal for portability"); # endif #endif #if @GNULIB_FMODF@ # if @REPLACE_FMODF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmodf # define fmodf rpl_fmodf # endif _GL_FUNCDECL_RPL (fmodf, float, (float x, float y)); _GL_CXXALIAS_RPL (fmodf, float, (float x, float y)); # else # if !@HAVE_FMODF@ # undef fmodf _GL_FUNCDECL_SYS (fmodf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (fmodf, float, (float x, float y)); # endif _GL_CXXALIASWARN (fmodf); #elif defined GNULIB_POSIXCHECK # undef fmodf # if HAVE_RAW_DECL_FMODF _GL_WARN_ON_USE (fmodf, "fmodf is unportable - " "use gnulib module fmodf for portability"); # endif #endif #if @GNULIB_FMOD@ # if @REPLACE_FMOD@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmod # define fmod rpl_fmod # endif _GL_FUNCDECL_RPL (fmod, double, (double x, double y)); _GL_CXXALIAS_RPL (fmod, double, (double x, double y)); # else _GL_CXXALIAS_SYS (fmod, double, (double x, double y)); # endif _GL_CXXALIASWARN (fmod); #elif defined GNULIB_POSIXCHECK # undef fmod # if HAVE_RAW_DECL_FMOD _GL_WARN_ON_USE (fmod, "fmod has portability problems - " "use gnulib module fmod for portability"); # endif #endif #if @GNULIB_FMODL@ # if @REPLACE_FMODL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef fmodl # define fmodl rpl_fmodl # endif _GL_FUNCDECL_RPL (fmodl, long double, (long double x, long double y)); _GL_CXXALIAS_RPL (fmodl, long double, (long double x, long double y)); # else # if !@HAVE_FMODL@ # undef fmodl _GL_FUNCDECL_SYS (fmodl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (fmodl, long double, (long double x, long double y)); # endif _GL_CXXALIASWARN (fmodl); #elif defined GNULIB_POSIXCHECK # undef fmodl # if HAVE_RAW_DECL_FMODL _GL_WARN_ON_USE (fmodl, "fmodl is unportable - " "use gnulib module fmodl for portability"); # endif #endif /* Write x as x = mantissa * 2^exp where If x finite and nonzero: 0.5 <= |mantissa| < 1.0. If x is zero: mantissa = x, exp = 0. If x is infinite or NaN: mantissa = x, exp unspecified. Store exp in *EXPPTR and return mantissa. */ #if @GNULIB_FREXPF@ # if @REPLACE_FREXPF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef frexpf # define frexpf rpl_frexpf # endif _GL_FUNCDECL_RPL (frexpf, float, (float x, int *expptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (frexpf, float, (float x, int *expptr)); # else # if !@HAVE_FREXPF@ # undef frexpf _GL_FUNCDECL_SYS (frexpf, float, (float x, int *expptr) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (frexpf, float, (float x, int *expptr)); # endif _GL_CXXALIASWARN (frexpf); #elif defined GNULIB_POSIXCHECK # undef frexpf # if HAVE_RAW_DECL_FREXPF _GL_WARN_ON_USE (frexpf, "frexpf is unportable - " "use gnulib module frexpf for portability"); # endif #endif /* Write x as x = mantissa * 2^exp where If x finite and nonzero: 0.5 <= |mantissa| < 1.0. If x is zero: mantissa = x, exp = 0. If x is infinite or NaN: mantissa = x, exp unspecified. Store exp in *EXPPTR and return mantissa. */ #if @GNULIB_FREXP@ # if @REPLACE_FREXP@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef frexp # define frexp rpl_frexp # endif _GL_FUNCDECL_RPL (frexp, double, (double x, int *expptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (frexp, double, (double x, int *expptr)); # else _GL_CXXALIAS_SYS (frexp, double, (double x, int *expptr)); # endif _GL_CXXALIASWARN1 (frexp, double, (double x, int *expptr)); #elif defined GNULIB_POSIXCHECK # undef frexp /* Assume frexp is always declared. */ _GL_WARN_ON_USE (frexp, "frexp is unportable - " "use gnulib module frexp for portability"); #endif /* Write x as x = mantissa * 2^exp where If x finite and nonzero: 0.5 <= |mantissa| < 1.0. If x is zero: mantissa = x, exp = 0. If x is infinite or NaN: mantissa = x, exp unspecified. Store exp in *EXPPTR and return mantissa. */ #if @GNULIB_FREXPL@ && @REPLACE_FREXPL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef frexpl # define frexpl rpl_frexpl # endif _GL_FUNCDECL_RPL (frexpl, long double, (long double x, int *expptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (frexpl, long double, (long double x, int *expptr)); #else # if !@HAVE_DECL_FREXPL@ _GL_FUNCDECL_SYS (frexpl, long double, (long double x, int *expptr) _GL_ARG_NONNULL ((2))); # endif # if @GNULIB_FREXPL@ _GL_CXXALIAS_SYS (frexpl, long double, (long double x, int *expptr)); # endif #endif #if @GNULIB_FREXPL@ && !(@REPLACE_FREXPL@ && !@HAVE_DECL_FREXPL@) _GL_CXXALIASWARN (frexpl); #endif #if !@GNULIB_FREXPL@ && defined GNULIB_POSIXCHECK # undef frexpl # if HAVE_RAW_DECL_FREXPL _GL_WARN_ON_USE (frexpl, "frexpl is unportable - " "use gnulib module frexpl for portability"); # endif #endif /* Return sqrt(x^2+y^2). */ #if @GNULIB_HYPOTF@ # if @REPLACE_HYPOTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef hypotf # define hypotf rpl_hypotf # endif _GL_FUNCDECL_RPL (hypotf, float, (float x, float y)); _GL_CXXALIAS_RPL (hypotf, float, (float x, float y)); # else # if !@HAVE_HYPOTF@ _GL_FUNCDECL_SYS (hypotf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (hypotf, float, (float x, float y)); # endif _GL_CXXALIASWARN (hypotf); #elif defined GNULIB_POSIXCHECK # undef hypotf # if HAVE_RAW_DECL_HYPOTF _GL_WARN_ON_USE (hypotf, "hypotf is unportable - " "use gnulib module hypotf for portability"); # endif #endif /* Return sqrt(x^2+y^2). */ #if @GNULIB_HYPOT@ # if @REPLACE_HYPOT@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef hypot # define hypot rpl_hypot # endif _GL_FUNCDECL_RPL (hypot, double, (double x, double y)); _GL_CXXALIAS_RPL (hypot, double, (double x, double y)); # else _GL_CXXALIAS_SYS (hypot, double, (double x, double y)); # endif _GL_CXXALIASWARN (hypot); #elif defined GNULIB_POSIXCHECK # undef hypot # if HAVE_RAW_DECL_HYPOT _GL_WARN_ON_USE (hypotf, "hypot has portability problems - " "use gnulib module hypot for portability"); # endif #endif /* Return sqrt(x^2+y^2). */ #if @GNULIB_HYPOTL@ # if @REPLACE_HYPOTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef hypotl # define hypotl rpl_hypotl # endif _GL_FUNCDECL_RPL (hypotl, long double, (long double x, long double y)); _GL_CXXALIAS_RPL (hypotl, long double, (long double x, long double y)); # else # if !@HAVE_HYPOTL@ _GL_FUNCDECL_SYS (hypotl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (hypotl, long double, (long double x, long double y)); # endif _GL_CXXALIASWARN (hypotl); #elif defined GNULIB_POSIXCHECK # undef hypotl # if HAVE_RAW_DECL_HYPOTL _GL_WARN_ON_USE (hypotl, "hypotl is unportable - " "use gnulib module hypotl for portability"); # endif #endif #if @GNULIB_ILOGBF@ # if @REPLACE_ILOGBF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ilogbf # define ilogbf rpl_ilogbf # endif _GL_FUNCDECL_RPL (ilogbf, int, (float x)); _GL_CXXALIAS_RPL (ilogbf, int, (float x)); # else # if !@HAVE_ILOGBF@ _GL_FUNCDECL_SYS (ilogbf, int, (float x)); # endif _GL_CXXALIAS_SYS (ilogbf, int, (float x)); # endif _GL_CXXALIASWARN (ilogbf); #elif defined GNULIB_POSIXCHECK # undef ilogbf # if HAVE_RAW_DECL_ILOGBF _GL_WARN_ON_USE (ilogbf, "ilogbf is unportable - " "use gnulib module ilogbf for portability"); # endif #endif #if @GNULIB_ILOGB@ # if @REPLACE_ILOGB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ilogb # define ilogb rpl_ilogb # endif _GL_FUNCDECL_RPL (ilogb, int, (double x)); _GL_CXXALIAS_RPL (ilogb, int, (double x)); # else # if !@HAVE_ILOGB@ _GL_FUNCDECL_SYS (ilogb, int, (double x)); # endif _GL_CXXALIAS_SYS (ilogb, int, (double x)); # endif _GL_CXXALIASWARN (ilogb); #elif defined GNULIB_POSIXCHECK # undef ilogb # if HAVE_RAW_DECL_ILOGB _GL_WARN_ON_USE (ilogb, "ilogb is unportable - " "use gnulib module ilogb for portability"); # endif #endif #if @GNULIB_ILOGBL@ # if @REPLACE_ILOGBL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ilogbl # define ilogbl rpl_ilogbl # endif _GL_FUNCDECL_RPL (ilogbl, int, (long double x)); _GL_CXXALIAS_RPL (ilogbl, int, (long double x)); # else # if !@HAVE_ILOGBL@ _GL_FUNCDECL_SYS (ilogbl, int, (long double x)); # endif _GL_CXXALIAS_SYS (ilogbl, int, (long double x)); # endif _GL_CXXALIASWARN (ilogbl); #elif defined GNULIB_POSIXCHECK # undef ilogbl # if HAVE_RAW_DECL_ILOGBL _GL_WARN_ON_USE (ilogbl, "ilogbl is unportable - " "use gnulib module ilogbl for portability"); # endif #endif /* Return x * 2^exp. */ #if @GNULIB_LDEXPF@ # if !@HAVE_LDEXPF@ # undef ldexpf _GL_FUNCDECL_SYS (ldexpf, float, (float x, int exp)); # endif _GL_CXXALIAS_SYS (ldexpf, float, (float x, int exp)); _GL_CXXALIASWARN (ldexpf); #elif defined GNULIB_POSIXCHECK # undef ldexpf # if HAVE_RAW_DECL_LDEXPF _GL_WARN_ON_USE (ldexpf, "ldexpf is unportable - " "use gnulib module ldexpf for portability"); # endif #endif /* Return x * 2^exp. */ #if @GNULIB_LDEXPL@ && @REPLACE_LDEXPL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef ldexpl # define ldexpl rpl_ldexpl # endif _GL_FUNCDECL_RPL (ldexpl, long double, (long double x, int exp)); _GL_CXXALIAS_RPL (ldexpl, long double, (long double x, int exp)); #else # if !@HAVE_DECL_LDEXPL@ _GL_FUNCDECL_SYS (ldexpl, long double, (long double x, int exp)); # endif # if @GNULIB_LDEXPL@ _GL_CXXALIAS_SYS (ldexpl, long double, (long double x, int exp)); # endif #endif #if @GNULIB_LDEXPL@ _GL_CXXALIASWARN (ldexpl); #endif #if !@GNULIB_LDEXPL@ && defined GNULIB_POSIXCHECK # undef ldexpl # if HAVE_RAW_DECL_LDEXPL _GL_WARN_ON_USE (ldexpl, "ldexpl is unportable - " "use gnulib module ldexpl for portability"); # endif #endif #if @GNULIB_LOGF@ # if @REPLACE_LOGF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logf # define logf rpl_logf # endif _GL_FUNCDECL_RPL (logf, float, (float x)); _GL_CXXALIAS_RPL (logf, float, (float x)); # else # if !@HAVE_LOGF@ # undef logf _GL_FUNCDECL_SYS (logf, float, (float x)); # endif _GL_CXXALIAS_SYS (logf, float, (float x)); # endif _GL_CXXALIASWARN (logf); #elif defined GNULIB_POSIXCHECK # undef logf # if HAVE_RAW_DECL_LOGF _GL_WARN_ON_USE (logf, "logf is unportable - " "use gnulib module logf for portability"); # endif #endif #if @GNULIB_LOG@ # if @REPLACE_LOG@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log # define log rpl_log # endif _GL_FUNCDECL_RPL (log, double, (double x)); _GL_CXXALIAS_RPL (log, double, (double x)); # else _GL_CXXALIAS_SYS (log, double, (double x)); # endif _GL_CXXALIASWARN (log); #elif defined GNULIB_POSIXCHECK # undef log # if HAVE_RAW_DECL_LOG _GL_WARN_ON_USE (log, "log has portability problems - " "use gnulib module log for portability"); # endif #endif #if @GNULIB_LOGL@ # if @REPLACE_LOGL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logl # define logl rpl_logl # endif _GL_FUNCDECL_RPL (logl, long double, (long double x)); _GL_CXXALIAS_RPL (logl, long double, (long double x)); # else # if !@HAVE_LOGL@ || !@HAVE_DECL_LOGL@ # undef logl _GL_FUNCDECL_SYS (logl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (logl, long double, (long double x)); # endif _GL_CXXALIASWARN (logl); #elif defined GNULIB_POSIXCHECK # undef logl # if HAVE_RAW_DECL_LOGL _GL_WARN_ON_USE (logl, "logl is unportable - " "use gnulib module logl for portability"); # endif #endif #if @GNULIB_LOG10F@ # if @REPLACE_LOG10F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log10f # define log10f rpl_log10f # endif _GL_FUNCDECL_RPL (log10f, float, (float x)); _GL_CXXALIAS_RPL (log10f, float, (float x)); # else # if !@HAVE_LOG10F@ # undef log10f _GL_FUNCDECL_SYS (log10f, float, (float x)); # endif _GL_CXXALIAS_SYS (log10f, float, (float x)); # endif _GL_CXXALIASWARN (log10f); #elif defined GNULIB_POSIXCHECK # undef log10f # if HAVE_RAW_DECL_LOG10F _GL_WARN_ON_USE (log10f, "log10f is unportable - " "use gnulib module log10f for portability"); # endif #endif #if @GNULIB_LOG10@ # if @REPLACE_LOG10@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log10 # define log10 rpl_log10 # endif _GL_FUNCDECL_RPL (log10, double, (double x)); _GL_CXXALIAS_RPL (log10, double, (double x)); # else _GL_CXXALIAS_SYS (log10, double, (double x)); # endif _GL_CXXALIASWARN (log10); #elif defined GNULIB_POSIXCHECK # undef log10 # if HAVE_RAW_DECL_LOG10 _GL_WARN_ON_USE (log10, "log10 has portability problems - " "use gnulib module log10 for portability"); # endif #endif #if @GNULIB_LOG10L@ # if @REPLACE_LOG10L@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log10l # define log10l rpl_log10l # endif _GL_FUNCDECL_RPL (log10l, long double, (long double x)); _GL_CXXALIAS_RPL (log10l, long double, (long double x)); # else # if !@HAVE_LOG10L@ || !@HAVE_DECL_LOG10L@ # undef log10l _GL_FUNCDECL_SYS (log10l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (log10l, long double, (long double x)); # endif _GL_CXXALIASWARN (log10l); #elif defined GNULIB_POSIXCHECK # undef log10l # if HAVE_RAW_DECL_LOG10L _GL_WARN_ON_USE (log10l, "log10l is unportable - " "use gnulib module log10l for portability"); # endif #endif #if @GNULIB_LOG1PF@ # if @REPLACE_LOG1PF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log1pf # define log1pf rpl_log1pf # endif _GL_FUNCDECL_RPL (log1pf, float, (float x)); _GL_CXXALIAS_RPL (log1pf, float, (float x)); # else # if !@HAVE_LOG1PF@ _GL_FUNCDECL_SYS (log1pf, float, (float x)); # endif _GL_CXXALIAS_SYS (log1pf, float, (float x)); # endif _GL_CXXALIASWARN (log1pf); #elif defined GNULIB_POSIXCHECK # undef log1pf # if HAVE_RAW_DECL_LOG1PF _GL_WARN_ON_USE (log1pf, "log1pf is unportable - " "use gnulib module log1pf for portability"); # endif #endif #if @GNULIB_LOG1P@ # if @REPLACE_LOG1P@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log1p # define log1p rpl_log1p # endif _GL_FUNCDECL_RPL (log1p, double, (double x)); _GL_CXXALIAS_RPL (log1p, double, (double x)); # else # if !@HAVE_LOG1P@ _GL_FUNCDECL_SYS (log1p, double, (double x)); # endif _GL_CXXALIAS_SYS (log1p, double, (double x)); # endif _GL_CXXALIASWARN (log1p); #elif defined GNULIB_POSIXCHECK # undef log1p # if HAVE_RAW_DECL_LOG1P _GL_WARN_ON_USE (log1p, "log1p has portability problems - " "use gnulib module log1p for portability"); # endif #endif #if @GNULIB_LOG1PL@ # if @REPLACE_LOG1PL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log1pl # define log1pl rpl_log1pl # endif _GL_FUNCDECL_RPL (log1pl, long double, (long double x)); _GL_CXXALIAS_RPL (log1pl, long double, (long double x)); # else # if !@HAVE_LOG1PL@ _GL_FUNCDECL_SYS (log1pl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (log1pl, long double, (long double x)); # endif _GL_CXXALIASWARN (log1pl); #elif defined GNULIB_POSIXCHECK # undef log1pl # if HAVE_RAW_DECL_LOG1PL _GL_WARN_ON_USE (log1pl, "log1pl has portability problems - " "use gnulib module log1pl for portability"); # endif #endif #if @GNULIB_LOG2F@ # if @REPLACE_LOG2F@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log2f # define log2f rpl_log2f # endif _GL_FUNCDECL_RPL (log2f, float, (float x)); _GL_CXXALIAS_RPL (log2f, float, (float x)); # else # if !@HAVE_DECL_LOG2F@ # undef log2f _GL_FUNCDECL_SYS (log2f, float, (float x)); # endif _GL_CXXALIAS_SYS (log2f, float, (float x)); # endif _GL_CXXALIASWARN (log2f); #elif defined GNULIB_POSIXCHECK # undef log2f # if HAVE_RAW_DECL_LOG2F _GL_WARN_ON_USE (log2f, "log2f is unportable - " "use gnulib module log2f for portability"); # endif #endif #if @GNULIB_LOG2@ # if @REPLACE_LOG2@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log2 # define log2 rpl_log2 # endif _GL_FUNCDECL_RPL (log2, double, (double x)); _GL_CXXALIAS_RPL (log2, double, (double x)); # else # if !@HAVE_DECL_LOG2@ # undef log2 _GL_FUNCDECL_SYS (log2, double, (double x)); # endif _GL_CXXALIAS_SYS (log2, double, (double x)); # endif _GL_CXXALIASWARN (log2); #elif defined GNULIB_POSIXCHECK # undef log2 # if HAVE_RAW_DECL_LOG2 _GL_WARN_ON_USE (log2, "log2 is unportable - " "use gnulib module log2 for portability"); # endif #endif #if @GNULIB_LOG2L@ # if @REPLACE_LOG2L@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef log2l # define log2l rpl_log2l # endif _GL_FUNCDECL_RPL (log2l, long double, (long double x)); _GL_CXXALIAS_RPL (log2l, long double, (long double x)); # else # if !@HAVE_DECL_LOG2L@ _GL_FUNCDECL_SYS (log2l, long double, (long double x)); # endif _GL_CXXALIAS_SYS (log2l, long double, (long double x)); # endif _GL_CXXALIASWARN (log2l); #elif defined GNULIB_POSIXCHECK # undef log2l # if HAVE_RAW_DECL_LOG2L _GL_WARN_ON_USE (log2l, "log2l is unportable - " "use gnulib module log2l for portability"); # endif #endif #if @GNULIB_LOGBF@ # if @REPLACE_LOGBF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logbf # define logbf rpl_logbf # endif _GL_FUNCDECL_RPL (logbf, float, (float x)); _GL_CXXALIAS_RPL (logbf, float, (float x)); # else # if !@HAVE_LOGBF@ _GL_FUNCDECL_SYS (logbf, float, (float x)); # endif _GL_CXXALIAS_SYS (logbf, float, (float x)); # endif _GL_CXXALIASWARN (logbf); #elif defined GNULIB_POSIXCHECK # undef logbf # if HAVE_RAW_DECL_LOGBF _GL_WARN_ON_USE (logbf, "logbf is unportable - " "use gnulib module logbf for portability"); # endif #endif #if @GNULIB_LOGB@ # if @REPLACE_LOGB@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logb # define logb rpl_logb # endif _GL_FUNCDECL_RPL (logb, double, (double x)); _GL_CXXALIAS_RPL (logb, double, (double x)); # else # if !@HAVE_DECL_LOGB@ _GL_FUNCDECL_SYS (logb, double, (double x)); # endif _GL_CXXALIAS_SYS (logb, double, (double x)); # endif _GL_CXXALIASWARN (logb); #elif defined GNULIB_POSIXCHECK # undef logb # if HAVE_RAW_DECL_LOGB _GL_WARN_ON_USE (logb, "logb is unportable - " "use gnulib module logb for portability"); # endif #endif #if @GNULIB_LOGBL@ # if @REPLACE_LOGBL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef logbl # define logbl rpl_logbl # endif _GL_FUNCDECL_RPL (logbl, long double, (long double x)); _GL_CXXALIAS_RPL (logbl, long double, (long double x)); # else # if !@HAVE_LOGBL@ _GL_FUNCDECL_SYS (logbl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (logbl, long double, (long double x)); # endif _GL_CXXALIASWARN (logbl); #elif defined GNULIB_POSIXCHECK # undef logbl # if HAVE_RAW_DECL_LOGBL _GL_WARN_ON_USE (logbl, "logbl is unportable - " "use gnulib module logbl for portability"); # endif #endif #if @GNULIB_MODFF@ # if @REPLACE_MODFF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef modff # define modff rpl_modff # endif _GL_FUNCDECL_RPL (modff, float, (float x, float *iptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (modff, float, (float x, float *iptr)); # else # if !@HAVE_MODFF@ # undef modff _GL_FUNCDECL_SYS (modff, float, (float x, float *iptr) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (modff, float, (float x, float *iptr)); # endif _GL_CXXALIASWARN (modff); #elif defined GNULIB_POSIXCHECK # undef modff # if HAVE_RAW_DECL_MODFF _GL_WARN_ON_USE (modff, "modff is unportable - " "use gnulib module modff for portability"); # endif #endif #if @GNULIB_MODF@ # if @REPLACE_MODF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef modf # define modf rpl_modf # endif _GL_FUNCDECL_RPL (modf, double, (double x, double *iptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (modf, double, (double x, double *iptr)); # else _GL_CXXALIAS_SYS (modf, double, (double x, double *iptr)); # endif _GL_CXXALIASWARN (modf); #elif defined GNULIB_POSIXCHECK # undef modf # if HAVE_RAW_DECL_MODF _GL_WARN_ON_USE (modf, "modf has portability problems - " "use gnulib module modf for portability"); # endif #endif #if @GNULIB_MODFL@ # if @REPLACE_MODFL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef modfl # define modfl rpl_modfl # endif _GL_FUNCDECL_RPL (modfl, long double, (long double x, long double *iptr) _GL_ARG_NONNULL ((2))); _GL_CXXALIAS_RPL (modfl, long double, (long double x, long double *iptr)); # else # if !@HAVE_MODFL@ # undef modfl _GL_FUNCDECL_SYS (modfl, long double, (long double x, long double *iptr) _GL_ARG_NONNULL ((2))); # endif _GL_CXXALIAS_SYS (modfl, long double, (long double x, long double *iptr)); # endif _GL_CXXALIASWARN (modfl); #elif defined GNULIB_POSIXCHECK # undef modfl # if HAVE_RAW_DECL_MODFL _GL_WARN_ON_USE (modfl, "modfl is unportable - " "use gnulib module modfl for portability"); # endif #endif #if @GNULIB_POWF@ # if !@HAVE_POWF@ # undef powf _GL_FUNCDECL_SYS (powf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (powf, float, (float x, float y)); _GL_CXXALIASWARN (powf); #elif defined GNULIB_POSIXCHECK # undef powf # if HAVE_RAW_DECL_POWF _GL_WARN_ON_USE (powf, "powf is unportable - " "use gnulib module powf for portability"); # endif #endif #if @GNULIB_REMAINDERF@ # if @REPLACE_REMAINDERF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remainderf # define remainderf rpl_remainderf # endif _GL_FUNCDECL_RPL (remainderf, float, (float x, float y)); _GL_CXXALIAS_RPL (remainderf, float, (float x, float y)); # else # if !@HAVE_REMAINDERF@ _GL_FUNCDECL_SYS (remainderf, float, (float x, float y)); # endif _GL_CXXALIAS_SYS (remainderf, float, (float x, float y)); # endif _GL_CXXALIASWARN (remainderf); #elif defined GNULIB_POSIXCHECK # undef remainderf # if HAVE_RAW_DECL_REMAINDERF _GL_WARN_ON_USE (remainderf, "remainderf is unportable - " "use gnulib module remainderf for portability"); # endif #endif #if @GNULIB_REMAINDER@ # if @REPLACE_REMAINDER@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remainder # define remainder rpl_remainder # endif _GL_FUNCDECL_RPL (remainder, double, (double x, double y)); _GL_CXXALIAS_RPL (remainder, double, (double x, double y)); # else # if !@HAVE_REMAINDER@ || !@HAVE_DECL_REMAINDER@ _GL_FUNCDECL_SYS (remainder, double, (double x, double y)); # endif _GL_CXXALIAS_SYS (remainder, double, (double x, double y)); # endif _GL_CXXALIASWARN (remainder); #elif defined GNULIB_POSIXCHECK # undef remainder # if HAVE_RAW_DECL_REMAINDER _GL_WARN_ON_USE (remainder, "remainder is unportable - " "use gnulib module remainder for portability"); # endif #endif #if @GNULIB_REMAINDERL@ # if @REPLACE_REMAINDERL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef remainderl # define remainderl rpl_remainderl # endif _GL_FUNCDECL_RPL (remainderl, long double, (long double x, long double y)); _GL_CXXALIAS_RPL (remainderl, long double, (long double x, long double y)); # else # if !@HAVE_DECL_REMAINDERL@ # undef remainderl _GL_FUNCDECL_SYS (remainderl, long double, (long double x, long double y)); # endif _GL_CXXALIAS_SYS (remainderl, long double, (long double x, long double y)); # endif _GL_CXXALIASWARN (remainderl); #elif defined GNULIB_POSIXCHECK # undef remainderl # if HAVE_RAW_DECL_REMAINDERL _GL_WARN_ON_USE (remainderl, "remainderl is unportable - " "use gnulib module remainderl for portability"); # endif #endif #if @GNULIB_RINTF@ # if !@HAVE_DECL_RINTF@ _GL_FUNCDECL_SYS (rintf, float, (float x)); # endif _GL_CXXALIAS_SYS (rintf, float, (float x)); _GL_CXXALIASWARN (rintf); #elif defined GNULIB_POSIXCHECK # undef rintf # if HAVE_RAW_DECL_RINTF _GL_WARN_ON_USE (rintf, "rintf is unportable - " "use gnulib module rintf for portability"); # endif #endif #if @GNULIB_RINT@ # if !@HAVE_RINT@ _GL_FUNCDECL_SYS (rint, double, (double x)); # endif _GL_CXXALIAS_SYS (rint, double, (double x)); _GL_CXXALIASWARN (rint); #elif defined GNULIB_POSIXCHECK # undef rint # if HAVE_RAW_DECL_RINT _GL_WARN_ON_USE (rint, "rint is unportable - " "use gnulib module rint for portability"); # endif #endif #if @GNULIB_RINTL@ # if !@HAVE_RINTL@ _GL_FUNCDECL_SYS (rintl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (rintl, long double, (long double x)); _GL_CXXALIASWARN (rintl); #elif defined GNULIB_POSIXCHECK # undef rintl # if HAVE_RAW_DECL_RINTL _GL_WARN_ON_USE (rintl, "rintl is unportable - " "use gnulib module rintl for portability"); # endif #endif #if @GNULIB_ROUNDF@ # if @REPLACE_ROUNDF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef roundf # define roundf rpl_roundf # endif _GL_FUNCDECL_RPL (roundf, float, (float x)); _GL_CXXALIAS_RPL (roundf, float, (float x)); # else # if !@HAVE_DECL_ROUNDF@ _GL_FUNCDECL_SYS (roundf, float, (float x)); # endif _GL_CXXALIAS_SYS (roundf, float, (float x)); # endif _GL_CXXALIASWARN (roundf); #elif defined GNULIB_POSIXCHECK # undef roundf # if HAVE_RAW_DECL_ROUNDF _GL_WARN_ON_USE (roundf, "roundf is unportable - " "use gnulib module roundf for portability"); # endif #endif #if @GNULIB_ROUND@ # if @REPLACE_ROUND@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef round # define round rpl_round # endif _GL_FUNCDECL_RPL (round, double, (double x)); _GL_CXXALIAS_RPL (round, double, (double x)); # else # if !@HAVE_DECL_ROUND@ _GL_FUNCDECL_SYS (round, double, (double x)); # endif _GL_CXXALIAS_SYS (round, double, (double x)); # endif _GL_CXXALIASWARN (round); #elif defined GNULIB_POSIXCHECK # undef round # if HAVE_RAW_DECL_ROUND _GL_WARN_ON_USE (round, "round is unportable - " "use gnulib module round for portability"); # endif #endif #if @GNULIB_ROUNDL@ # if @REPLACE_ROUNDL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef roundl # define roundl rpl_roundl # endif _GL_FUNCDECL_RPL (roundl, long double, (long double x)); _GL_CXXALIAS_RPL (roundl, long double, (long double x)); # else # if !@HAVE_DECL_ROUNDL@ # undef roundl _GL_FUNCDECL_SYS (roundl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (roundl, long double, (long double x)); # endif _GL_CXXALIASWARN (roundl); #elif defined GNULIB_POSIXCHECK # undef roundl # if HAVE_RAW_DECL_ROUNDL _GL_WARN_ON_USE (roundl, "roundl is unportable - " "use gnulib module roundl for portability"); # endif #endif #if @GNULIB_SINF@ # if @REPLACE_SINF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sinf # define sinf rpl_sinf # endif _GL_FUNCDECL_RPL (sinf, float, (float x)); _GL_CXXALIAS_RPL (sinf, float, (float x)); # else # if !@HAVE_SINF@ # undef sinf _GL_FUNCDECL_SYS (sinf, float, (float x)); # endif _GL_CXXALIAS_SYS (sinf, float, (float x)); # endif _GL_CXXALIASWARN (sinf); #elif defined GNULIB_POSIXCHECK # undef sinf # if HAVE_RAW_DECL_SINF _GL_WARN_ON_USE (sinf, "sinf is unportable - " "use gnulib module sinf for portability"); # endif #endif #if @GNULIB_SINL@ # if !@HAVE_SINL@ || !@HAVE_DECL_SINL@ # undef sinl _GL_FUNCDECL_SYS (sinl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (sinl, long double, (long double x)); _GL_CXXALIASWARN (sinl); #elif defined GNULIB_POSIXCHECK # undef sinl # if HAVE_RAW_DECL_SINL _GL_WARN_ON_USE (sinl, "sinl is unportable - " "use gnulib module sinl for portability"); # endif #endif #if @GNULIB_SINHF@ # if @REPLACE_SINHF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sinhf # define sinhf rpl_sinhf # endif _GL_FUNCDECL_RPL (sinhf, float, (float x)); _GL_CXXALIAS_RPL (sinhf, float, (float x)); # else # if !@HAVE_SINHF@ # undef sinhf _GL_FUNCDECL_SYS (sinhf, float, (float x)); # endif _GL_CXXALIAS_SYS (sinhf, float, (float x)); # endif _GL_CXXALIASWARN (sinhf); #elif defined GNULIB_POSIXCHECK # undef sinhf # if HAVE_RAW_DECL_SINHF _GL_WARN_ON_USE (sinhf, "sinhf is unportable - " "use gnulib module sinhf for portability"); # endif #endif #if @GNULIB_SQRTF@ # if @REPLACE_SQRTF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sqrtf # define sqrtf rpl_sqrtf # endif _GL_FUNCDECL_RPL (sqrtf, float, (float x)); _GL_CXXALIAS_RPL (sqrtf, float, (float x)); # else # if !@HAVE_SQRTF@ # undef sqrtf _GL_FUNCDECL_SYS (sqrtf, float, (float x)); # endif _GL_CXXALIAS_SYS (sqrtf, float, (float x)); # endif _GL_CXXALIASWARN (sqrtf); #elif defined GNULIB_POSIXCHECK # undef sqrtf # if HAVE_RAW_DECL_SQRTF _GL_WARN_ON_USE (sqrtf, "sqrtf is unportable - " "use gnulib module sqrtf for portability"); # endif #endif #if @GNULIB_SQRTL@ # if @REPLACE_SQRTL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef sqrtl # define sqrtl rpl_sqrtl # endif _GL_FUNCDECL_RPL (sqrtl, long double, (long double x)); _GL_CXXALIAS_RPL (sqrtl, long double, (long double x)); # else # if !@HAVE_SQRTL@ || !@HAVE_DECL_SQRTL@ # undef sqrtl _GL_FUNCDECL_SYS (sqrtl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (sqrtl, long double, (long double x)); # endif _GL_CXXALIASWARN (sqrtl); #elif defined GNULIB_POSIXCHECK # undef sqrtl # if HAVE_RAW_DECL_SQRTL _GL_WARN_ON_USE (sqrtl, "sqrtl is unportable - " "use gnulib module sqrtl for portability"); # endif #endif #if @GNULIB_TANF@ # if @REPLACE_TANF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef tanf # define tanf rpl_tanf # endif _GL_FUNCDECL_RPL (tanf, float, (float x)); _GL_CXXALIAS_RPL (tanf, float, (float x)); # else # if !@HAVE_TANF@ # undef tanf _GL_FUNCDECL_SYS (tanf, float, (float x)); # endif _GL_CXXALIAS_SYS (tanf, float, (float x)); # endif _GL_CXXALIASWARN (tanf); #elif defined GNULIB_POSIXCHECK # undef tanf # if HAVE_RAW_DECL_TANF _GL_WARN_ON_USE (tanf, "tanf is unportable - " "use gnulib module tanf for portability"); # endif #endif #if @GNULIB_TANL@ # if !@HAVE_TANL@ || !@HAVE_DECL_TANL@ # undef tanl _GL_FUNCDECL_SYS (tanl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (tanl, long double, (long double x)); _GL_CXXALIASWARN (tanl); #elif defined GNULIB_POSIXCHECK # undef tanl # if HAVE_RAW_DECL_TANL _GL_WARN_ON_USE (tanl, "tanl is unportable - " "use gnulib module tanl for portability"); # endif #endif #if @GNULIB_TANHF@ # if @REPLACE_TANHF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef tanhf # define tanhf rpl_tanhf # endif _GL_FUNCDECL_RPL (tanhf, float, (float x)); _GL_CXXALIAS_RPL (tanhf, float, (float x)); # else # if !@HAVE_TANHF@ # undef tanhf _GL_FUNCDECL_SYS (tanhf, float, (float x)); # endif _GL_CXXALIAS_SYS (tanhf, float, (float x)); # endif _GL_CXXALIASWARN (tanhf); #elif defined GNULIB_POSIXCHECK # undef tanhf # if HAVE_RAW_DECL_TANHF _GL_WARN_ON_USE (tanhf, "tanhf is unportable - " "use gnulib module tanhf for portability"); # endif #endif #if @GNULIB_TRUNCF@ # if @REPLACE_TRUNCF@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef truncf # define truncf rpl_truncf # endif _GL_FUNCDECL_RPL (truncf, float, (float x)); _GL_CXXALIAS_RPL (truncf, float, (float x)); # else # if !@HAVE_DECL_TRUNCF@ _GL_FUNCDECL_SYS (truncf, float, (float x)); # endif _GL_CXXALIAS_SYS (truncf, float, (float x)); # endif _GL_CXXALIASWARN (truncf); #elif defined GNULIB_POSIXCHECK # undef truncf # if HAVE_RAW_DECL_TRUNCF _GL_WARN_ON_USE (truncf, "truncf is unportable - " "use gnulib module truncf for portability"); # endif #endif #if @GNULIB_TRUNC@ # if @REPLACE_TRUNC@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef trunc # define trunc rpl_trunc # endif _GL_FUNCDECL_RPL (trunc, double, (double x)); _GL_CXXALIAS_RPL (trunc, double, (double x)); # else # if !@HAVE_DECL_TRUNC@ _GL_FUNCDECL_SYS (trunc, double, (double x)); # endif _GL_CXXALIAS_SYS (trunc, double, (double x)); # endif _GL_CXXALIASWARN (trunc); #elif defined GNULIB_POSIXCHECK # undef trunc # if HAVE_RAW_DECL_TRUNC _GL_WARN_ON_USE (trunc, "trunc is unportable - " "use gnulib module trunc for portability"); # endif #endif #if @GNULIB_TRUNCL@ # if @REPLACE_TRUNCL@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef truncl # define truncl rpl_truncl # endif _GL_FUNCDECL_RPL (truncl, long double, (long double x)); _GL_CXXALIAS_RPL (truncl, long double, (long double x)); # else # if !@HAVE_DECL_TRUNCL@ _GL_FUNCDECL_SYS (truncl, long double, (long double x)); # endif _GL_CXXALIAS_SYS (truncl, long double, (long double x)); # endif _GL_CXXALIASWARN (truncl); #elif defined GNULIB_POSIXCHECK # undef truncl # if HAVE_RAW_DECL_TRUNCL _GL_WARN_ON_USE (truncl, "truncl is unportable - " "use gnulib module truncl for portability"); # endif #endif /* Definitions of function-like macros come here, after the function declarations. */ #if @GNULIB_ISFINITE@ # if @REPLACE_ISFINITE@ _GL_EXTERN_C int gl_isfinitef (float x); _GL_EXTERN_C int gl_isfinited (double x); _GL_EXTERN_C int gl_isfinitel (long double x); # undef isfinite # define isfinite(x) \ (sizeof (x) == sizeof (long double) ? gl_isfinitel (x) : \ sizeof (x) == sizeof (double) ? gl_isfinited (x) : \ gl_isfinitef (x)) # endif # ifdef __cplusplus # if defined isfinite || defined GNULIB_NAMESPACE _GL_MATH_CXX_REAL_FLOATING_DECL_1 (isfinite) # undef isfinite _GL_MATH_CXX_REAL_FLOATING_DECL_2 (isfinite) # endif # endif #elif defined GNULIB_POSIXCHECK # if defined isfinite _GL_WARN_REAL_FLOATING_DECL (isfinite); # undef isfinite # define isfinite(x) _GL_WARN_REAL_FLOATING_IMPL (isfinite, x) # endif #endif #if @GNULIB_ISINF@ # if @REPLACE_ISINF@ _GL_EXTERN_C int gl_isinff (float x); _GL_EXTERN_C int gl_isinfd (double x); _GL_EXTERN_C int gl_isinfl (long double x); # undef isinf # define isinf(x) \ (sizeof (x) == sizeof (long double) ? gl_isinfl (x) : \ sizeof (x) == sizeof (double) ? gl_isinfd (x) : \ gl_isinff (x)) # endif # ifdef __cplusplus # if defined isinf || defined GNULIB_NAMESPACE _GL_MATH_CXX_REAL_FLOATING_DECL_1 (isinf) # undef isinf _GL_MATH_CXX_REAL_FLOATING_DECL_2 (isinf) # endif # endif #elif defined GNULIB_POSIXCHECK # if defined isinf _GL_WARN_REAL_FLOATING_DECL (isinf); # undef isinf # define isinf(x) _GL_WARN_REAL_FLOATING_IMPL (isinf, x) # endif #endif #if @GNULIB_ISNANF@ /* Test for NaN for 'float' numbers. */ # if @HAVE_ISNANF@ /* The original included above provides a declaration of isnan macro or (older) isnanf function. */ # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) # elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) # endif # else /* Test whether X is a NaN. */ # undef isnanf # define isnanf rpl_isnanf _GL_EXTERN_C int isnanf (float x); # endif #endif #if @GNULIB_ISNAND@ /* Test for NaN for 'double' numbers. This function is a gnulib extension, unlike isnan() which applied only to 'double' numbers earlier but now is a type-generic macro. */ # if @HAVE_ISNAND@ /* The original included above provides a declaration of isnan macro. */ # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnand # define isnand(x) __builtin_isnan ((double)(x)) # else # undef isnand # define isnand(x) isnan ((double)(x)) # endif # else /* Test whether X is a NaN. */ # undef isnand # define isnand rpl_isnand _GL_EXTERN_C int isnand (double x); # endif #endif #if @GNULIB_ISNANL@ /* Test for NaN for 'long double' numbers. */ # if @HAVE_ISNANL@ /* The original included above provides a declaration of isnan macro or (older) isnanl function. */ # if __GNUC__ >= 4 /* GCC 4.0 and newer provides three built-ins for isnan. */ # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) # elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) # endif # else /* Test whether X is a NaN. */ # undef isnanl # define isnanl rpl_isnanl _GL_EXTERN_C int isnanl (long double x) _GL_ATTRIBUTE_CONST; # endif #endif /* This must come *after* the snippets for GNULIB_ISNANF and GNULIB_ISNANL! */ #if @GNULIB_ISNAN@ # if @REPLACE_ISNAN@ /* We can't just use the isnanf macro (e.g.) as exposed by isnanf.h (e.g.) here, because those may end up being macros that recursively expand back to isnan. So use the gnulib replacements for them directly. */ # if @HAVE_ISNANF@ && __GNUC__ >= 4 # define gl_isnan_f(x) __builtin_isnanf ((float)(x)) # else _GL_EXTERN_C int rpl_isnanf (float x); # define gl_isnan_f(x) rpl_isnanf (x) # endif # if @HAVE_ISNAND@ && __GNUC__ >= 4 # define gl_isnan_d(x) __builtin_isnan ((double)(x)) # else _GL_EXTERN_C int rpl_isnand (double x); # define gl_isnan_d(x) rpl_isnand (x) # endif # if @HAVE_ISNANL@ && __GNUC__ >= 4 # define gl_isnan_l(x) __builtin_isnanl ((long double)(x)) # else _GL_EXTERN_C int rpl_isnanl (long double x) _GL_ATTRIBUTE_CONST; # define gl_isnan_l(x) rpl_isnanl (x) # endif # undef isnan # define isnan(x) \ (sizeof (x) == sizeof (long double) ? gl_isnan_l (x) : \ sizeof (x) == sizeof (double) ? gl_isnan_d (x) : \ gl_isnan_f (x)) # elif __GNUC__ >= 4 # undef isnan # define isnan(x) \ (sizeof (x) == sizeof (long double) ? __builtin_isnanl ((long double)(x)) : \ sizeof (x) == sizeof (double) ? __builtin_isnan ((double)(x)) : \ __builtin_isnanf ((float)(x))) # endif # ifdef __cplusplus # if defined isnan || defined GNULIB_NAMESPACE _GL_MATH_CXX_REAL_FLOATING_DECL_1 (isnan) # undef isnan _GL_MATH_CXX_REAL_FLOATING_DECL_2 (isnan) # endif # else /* Ensure isnan is a macro. */ # ifndef isnan # define isnan isnan # endif # endif #elif defined GNULIB_POSIXCHECK # if defined isnan _GL_WARN_REAL_FLOATING_DECL (isnan); # undef isnan # define isnan(x) _GL_WARN_REAL_FLOATING_IMPL (isnan, x) # endif #endif #if @GNULIB_SIGNBIT@ # if (@REPLACE_SIGNBIT_USING_GCC@ \ && (!defined __cplusplus || __cplusplus < 201103)) # undef signbit /* GCC 4.0 and newer provides three built-ins for signbit. */ # define signbit(x) \ (sizeof (x) == sizeof (long double) ? __builtin_signbitl (x) : \ sizeof (x) == sizeof (double) ? __builtin_signbit (x) : \ __builtin_signbitf (x)) # endif # if @REPLACE_SIGNBIT@ # undef signbit _GL_EXTERN_C int gl_signbitf (float arg); _GL_EXTERN_C int gl_signbitd (double arg); _GL_EXTERN_C int gl_signbitl (long double arg); # if __GNUC__ >= 2 && !defined __STRICT_ANSI__ # define _GL_NUM_UINT_WORDS(type) \ ((sizeof (type) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) # if defined FLT_SIGNBIT_WORD && defined FLT_SIGNBIT_BIT && !defined gl_signbitf # define gl_signbitf_OPTIMIZED_MACRO # define gl_signbitf(arg) \ ({ union { float _value; \ unsigned int _word[_GL_NUM_UINT_WORDS (float)]; \ } _m; \ _m._value = (arg); \ (_m._word[FLT_SIGNBIT_WORD] >> FLT_SIGNBIT_BIT) & 1; \ }) # endif # if defined DBL_SIGNBIT_WORD && defined DBL_SIGNBIT_BIT && !defined gl_signbitd # define gl_signbitd_OPTIMIZED_MACRO # define gl_signbitd(arg) \ ({ union { double _value; \ unsigned int _word[_GL_NUM_UINT_WORDS (double)]; \ } _m; \ _m._value = (arg); \ (_m._word[DBL_SIGNBIT_WORD] >> DBL_SIGNBIT_BIT) & 1; \ }) # endif # if defined LDBL_SIGNBIT_WORD && defined LDBL_SIGNBIT_BIT && !defined gl_signbitl # define gl_signbitl_OPTIMIZED_MACRO # define gl_signbitl(arg) \ ({ union { long double _value; \ unsigned int _word[_GL_NUM_UINT_WORDS (long double)]; \ } _m; \ _m._value = (arg); \ (_m._word[LDBL_SIGNBIT_WORD] >> LDBL_SIGNBIT_BIT) & 1; \ }) # endif # endif # define signbit(x) \ (sizeof (x) == sizeof (long double) ? gl_signbitl (x) : \ sizeof (x) == sizeof (double) ? gl_signbitd (x) : \ gl_signbitf (x)) # endif # ifdef __cplusplus # if defined signbit || defined GNULIB_NAMESPACE _GL_MATH_CXX_REAL_FLOATING_DECL_1 (signbit) # undef signbit _GL_MATH_CXX_REAL_FLOATING_DECL_2 (signbit) # endif # endif #elif defined GNULIB_POSIXCHECK # if defined signbit _GL_WARN_REAL_FLOATING_DECL (signbit); # undef signbit # define signbit(x) _GL_WARN_REAL_FLOATING_IMPL (signbit, x) # endif #endif _GL_INLINE_HEADER_END #endif /* _@GUARD_PREFIX@_MATH_H */ #endif /* _@GUARD_PREFIX@_MATH_H */ gnuastro-0.5/bootstrapped/lib/locale.in.h0000644000175000017500000001600313217200021015416 00000000000000/* A POSIX . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ #ifdef _GL_ALREADY_INCLUDING_LOCALE_H /* Special invocation conventions to handle Solaris header files (through Solaris 10) when combined with gettext's libintl.h. */ #@INCLUDE_NEXT@ @NEXT_LOCALE_H@ #else /* Normal invocation convention. */ #ifndef _@GUARD_PREFIX@_LOCALE_H #define _GL_ALREADY_INCLUDING_LOCALE_H /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_LOCALE_H@ #undef _GL_ALREADY_INCLUDING_LOCALE_H #ifndef _@GUARD_PREFIX@_LOCALE_H #define _@GUARD_PREFIX@_LOCALE_H /* NetBSD 5.0 mis-defines NULL. */ #include /* Mac OS X 10.5 defines the locale_t type in . */ #if @HAVE_XLOCALE_H@ # include #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* The LC_MESSAGES locale category is specified in POSIX, but not in ISO C. On systems that don't define it, use the same value as GNU libintl. */ #if !defined LC_MESSAGES # define LC_MESSAGES 1729 #endif /* Bionic libc's 'struct lconv' is just a dummy. */ #if @REPLACE_STRUCT_LCONV@ # define lconv rpl_lconv struct lconv { /* All 'char *' are actually 'const char *'. */ /* Members that depend on the LC_NUMERIC category of the locale. See */ /* Symbol used as decimal point. */ char *decimal_point; /* Symbol used to separate groups of digits to the left of the decimal point. */ char *thousands_sep; /* Definition of the size of groups of digits to the left of the decimal point. */ char *grouping; /* Members that depend on the LC_MONETARY category of the locale. See */ /* Symbol used as decimal point. */ char *mon_decimal_point; /* Symbol used to separate groups of digits to the left of the decimal point. */ char *mon_thousands_sep; /* Definition of the size of groups of digits to the left of the decimal point. */ char *mon_grouping; /* Sign used to indicate a value >= 0. */ char *positive_sign; /* Sign used to indicate a value < 0. */ char *negative_sign; /* For formatting local currency. */ /* Currency symbol (3 characters) followed by separator (1 character). */ char *currency_symbol; /* Number of digits after the decimal point. */ char frac_digits; /* For values >= 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char p_cs_precedes; /* For values >= 0: Position of the sign. */ char p_sign_posn; /* For values >= 0: Placement of spaces between currency symbol, sign, and number. */ char p_sep_by_space; /* For values < 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char n_cs_precedes; /* For values < 0: Position of the sign. */ char n_sign_posn; /* For values < 0: Placement of spaces between currency symbol, sign, and number. */ char n_sep_by_space; /* For formatting international currency. */ /* Currency symbol (3 characters) followed by separator (1 character). */ char *int_curr_symbol; /* Number of digits after the decimal point. */ char int_frac_digits; /* For values >= 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char int_p_cs_precedes; /* For values >= 0: Position of the sign. */ char int_p_sign_posn; /* For values >= 0: Placement of spaces between currency symbol, sign, and number. */ char int_p_sep_by_space; /* For values < 0: 1 if the currency symbol precedes the number, 0 if it comes after the number. */ char int_n_cs_precedes; /* For values < 0: Position of the sign. */ char int_n_sign_posn; /* For values < 0: Placement of spaces between currency symbol, sign, and number. */ char int_n_sep_by_space; }; #endif #if @GNULIB_LOCALECONV@ # if @REPLACE_LOCALECONV@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef localeconv # define localeconv rpl_localeconv # endif _GL_FUNCDECL_RPL (localeconv, struct lconv *, (void)); _GL_CXXALIAS_RPL (localeconv, struct lconv *, (void)); # else _GL_CXXALIAS_SYS (localeconv, struct lconv *, (void)); # endif _GL_CXXALIASWARN (localeconv); #elif @REPLACE_STRUCT_LCONV@ # undef localeconv # define localeconv localeconv_used_without_requesting_gnulib_module_localeconv #elif defined GNULIB_POSIXCHECK # undef localeconv # if HAVE_RAW_DECL_LOCALECONV _GL_WARN_ON_USE (localeconv, "localeconv returns too few information on some platforms - " "use gnulib module localeconv for portability"); # endif #endif #if @GNULIB_SETLOCALE@ # if @REPLACE_SETLOCALE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef setlocale # define setlocale rpl_setlocale # define GNULIB_defined_setlocale 1 # endif _GL_FUNCDECL_RPL (setlocale, char *, (int category, const char *locale)); _GL_CXXALIAS_RPL (setlocale, char *, (int category, const char *locale)); # else _GL_CXXALIAS_SYS (setlocale, char *, (int category, const char *locale)); # endif _GL_CXXALIASWARN (setlocale); #elif defined GNULIB_POSIXCHECK # undef setlocale # if HAVE_RAW_DECL_SETLOCALE _GL_WARN_ON_USE (setlocale, "setlocale works differently on native Windows - " "use gnulib module setlocale for portability"); # endif #endif #if @GNULIB_DUPLOCALE@ # if @REPLACE_DUPLOCALE@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef duplocale # define duplocale rpl_duplocale # endif _GL_FUNCDECL_RPL (duplocale, locale_t, (locale_t locale) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (duplocale, locale_t, (locale_t locale)); # else # if @HAVE_DUPLOCALE@ _GL_CXXALIAS_SYS (duplocale, locale_t, (locale_t locale)); # endif # endif # if @HAVE_DUPLOCALE@ _GL_CXXALIASWARN (duplocale); # endif #elif defined GNULIB_POSIXCHECK # undef duplocale # if HAVE_RAW_DECL_DUPLOCALE _GL_WARN_ON_USE (duplocale, "duplocale is buggy on some glibc systems - " "use gnulib module duplocale for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_LOCALE_H */ #endif /* ! _GL_ALREADY_INCLUDING_LOCALE_H */ #endif /* _@GUARD_PREFIX@_LOCALE_H */ gnuastro-0.5/bootstrapped/lib/ref-del.sin0000644000175000017500000000167613217200021015444 00000000000000# Remove this package from a list of references stored in a text file. # # Copyright (C) 2000, 2009-2017 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, see . # # Written by Bruno Haible . # /^# Packages using this file: / { s/# Packages using this file:// s/ @PACKAGE@ / / s/^/# Packages using this file:/ } gnuastro-0.5/bootstrapped/lib/ref-add.sin0000644000175000017500000000175313217200021015424 00000000000000# Add this package to a list of references stored in a text file. # # Copyright (C) 2000, 2009-2017 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, see . # # Written by Bruno Haible . # /^# Packages using this file: / { s/# Packages using this file:// ta :a s/ @PACKAGE@ / @PACKAGE@ / tb s/ $/ @PACKAGE@ / :b s/^/# Packages using this file:/ } gnuastro-0.5/bootstrapped/lib/config.charset0000644000175000017500000005473713217200021016241 00000000000000#! /bin/sh # Output a system dependent table of character encoding aliases. # # Copyright (C) 2000-2004, 2006-2017 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, see . # # The table consists of lines of the form # ALIAS CANONICAL # # ALIAS is the (system dependent) result of "nl_langinfo (CODESET)". # ALIAS is compared in a case sensitive way. # # CANONICAL is the GNU canonical name for this character encoding. # It must be an encoding supported by libiconv. Support by GNU libc is # also desirable. CANONICAL is case insensitive. Usually an upper case # MIME charset name is preferred. # The current list of GNU canonical charset names is as follows. # # name MIME? used by which systems # (darwin = Mac OS X, woe32 = native Windows) # # ASCII, ANSI_X3.4-1968 glibc solaris freebsd netbsd darwin cygwin # ISO-8859-1 Y glibc aix hpux irix osf solaris freebsd netbsd openbsd darwin cygwin # ISO-8859-2 Y glibc aix hpux irix osf solaris freebsd netbsd openbsd darwin cygwin # ISO-8859-3 Y glibc solaris cygwin # ISO-8859-4 Y osf solaris freebsd netbsd openbsd darwin # ISO-8859-5 Y glibc aix hpux irix osf solaris freebsd netbsd openbsd darwin cygwin # ISO-8859-6 Y glibc aix hpux solaris cygwin # ISO-8859-7 Y glibc aix hpux irix osf solaris netbsd openbsd darwin cygwin # ISO-8859-8 Y glibc aix hpux osf solaris cygwin # ISO-8859-9 Y glibc aix hpux irix osf solaris darwin cygwin # ISO-8859-13 glibc netbsd openbsd darwin cygwin # ISO-8859-14 glibc cygwin # ISO-8859-15 glibc aix osf solaris freebsd netbsd openbsd darwin cygwin # KOI8-R Y glibc solaris freebsd netbsd openbsd darwin # KOI8-U Y glibc freebsd netbsd openbsd darwin cygwin # KOI8-T glibc # CP437 dos # CP775 dos # CP850 aix osf dos # CP852 dos # CP855 dos # CP856 aix # CP857 dos # CP861 dos # CP862 dos # CP864 dos # CP865 dos # CP866 freebsd netbsd openbsd darwin dos # CP869 dos # CP874 woe32 dos # CP922 aix # CP932 aix cygwin woe32 dos # CP943 aix # CP949 osf darwin woe32 dos # CP950 woe32 dos # CP1046 aix # CP1124 aix # CP1125 dos # CP1129 aix # CP1131 darwin # CP1250 woe32 # CP1251 glibc solaris netbsd openbsd darwin cygwin woe32 # CP1252 aix woe32 # CP1253 woe32 # CP1254 woe32 # CP1255 glibc woe32 # CP1256 woe32 # CP1257 woe32 # GB2312 Y glibc aix hpux irix solaris freebsd netbsd darwin # EUC-JP Y glibc aix hpux irix osf solaris freebsd netbsd darwin # EUC-KR Y glibc aix hpux irix osf solaris freebsd netbsd darwin cygwin # EUC-TW glibc aix hpux irix osf solaris netbsd # BIG5 Y glibc aix hpux osf solaris freebsd netbsd darwin cygwin # BIG5-HKSCS glibc solaris darwin # GBK glibc aix osf solaris darwin cygwin woe32 dos # GB18030 glibc solaris netbsd darwin # SHIFT_JIS Y hpux osf solaris freebsd netbsd darwin # JOHAB glibc solaris woe32 # TIS-620 glibc aix hpux osf solaris cygwin # VISCII Y glibc # TCVN5712-1 glibc # ARMSCII-8 glibc darwin # GEORGIAN-PS glibc cygwin # PT154 glibc # HP-ROMAN8 hpux # HP-ARABIC8 hpux # HP-GREEK8 hpux # HP-HEBREW8 hpux # HP-TURKISH8 hpux # HP-KANA8 hpux # DEC-KANJI osf # DEC-HANYU osf # UTF-8 Y glibc aix hpux osf solaris netbsd darwin cygwin # # Note: Names which are not marked as being a MIME name should not be used in # Internet protocols for information interchange (mail, news, etc.). # # Note: ASCII and ANSI_X3.4-1968 are synonymous canonical names. Applications # must understand both names and treat them as equivalent. # # The first argument passed to this file is the canonical host specification, # CPU_TYPE-MANUFACTURER-OPERATING_SYSTEM # or # CPU_TYPE-MANUFACTURER-KERNEL-OPERATING_SYSTEM host="$1" os=`echo "$host" | sed -e 's/^[^-]*-[^-]*-\(.*\)$/\1/'` echo "# This file contains a table of character encoding aliases," echo "# suitable for operating system '${os}'." echo "# It was automatically generated from config.charset." # List of references, updated during installation: echo "# Packages using this file: " case "$os" in linux-gnulibc1*) # Linux libc5 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "C ASCII" echo "POSIX ASCII" for l in af af_ZA ca ca_ES da da_DK de de_AT de_BE de_CH de_DE de_LU \ en en_AU en_BW en_CA en_DK en_GB en_IE en_NZ en_US en_ZA \ en_ZW es es_AR es_BO es_CL es_CO es_DO es_EC es_ES es_GT \ es_HN es_MX es_PA es_PE es_PY es_SV es_US es_UY es_VE et \ et_EE eu eu_ES fi fi_FI fo fo_FO fr fr_BE fr_CA fr_CH fr_FR \ fr_LU ga ga_IE gl gl_ES id id_ID in in_ID is is_IS it it_CH \ it_IT kl kl_GL nl nl_BE nl_NL no no_NO pt pt_BR pt_PT sv \ sv_FI sv_SE; do echo "$l ISO-8859-1" echo "$l.iso-8859-1 ISO-8859-1" echo "$l.iso-8859-15 ISO-8859-15" echo "$l.iso-8859-15@euro ISO-8859-15" echo "$l@euro ISO-8859-15" echo "$l.cp-437 CP437" echo "$l.cp-850 CP850" echo "$l.cp-1252 CP1252" echo "$l.cp-1252@euro CP1252" #echo "$l.atari-st ATARI-ST" # not a commonly used encoding echo "$l.utf-8 UTF-8" echo "$l.utf-8@euro UTF-8" done for l in cs cs_CZ hr hr_HR hu hu_HU pl pl_PL ro ro_RO sk sk_SK sl \ sl_SI sr sr_CS sr_YU; do echo "$l ISO-8859-2" echo "$l.iso-8859-2 ISO-8859-2" echo "$l.cp-852 CP852" echo "$l.cp-1250 CP1250" echo "$l.utf-8 UTF-8" done for l in mk mk_MK ru ru_RU; do echo "$l ISO-8859-5" echo "$l.iso-8859-5 ISO-8859-5" echo "$l.koi8-r KOI8-R" echo "$l.cp-866 CP866" echo "$l.cp-1251 CP1251" echo "$l.utf-8 UTF-8" done for l in ar ar_SA; do echo "$l ISO-8859-6" echo "$l.iso-8859-6 ISO-8859-6" echo "$l.cp-864 CP864" #echo "$l.cp-868 CP868" # not a commonly used encoding echo "$l.cp-1256 CP1256" echo "$l.utf-8 UTF-8" done for l in el el_GR gr gr_GR; do echo "$l ISO-8859-7" echo "$l.iso-8859-7 ISO-8859-7" echo "$l.cp-869 CP869" echo "$l.cp-1253 CP1253" echo "$l.cp-1253@euro CP1253" echo "$l.utf-8 UTF-8" echo "$l.utf-8@euro UTF-8" done for l in he he_IL iw iw_IL; do echo "$l ISO-8859-8" echo "$l.iso-8859-8 ISO-8859-8" echo "$l.cp-862 CP862" echo "$l.cp-1255 CP1255" echo "$l.utf-8 UTF-8" done for l in tr tr_TR; do echo "$l ISO-8859-9" echo "$l.iso-8859-9 ISO-8859-9" echo "$l.cp-857 CP857" echo "$l.cp-1254 CP1254" echo "$l.utf-8 UTF-8" done for l in lt lt_LT lv lv_LV; do #echo "$l BALTIC" # not a commonly used encoding, wrong encoding name echo "$l ISO-8859-13" done for l in ru_UA uk uk_UA; do echo "$l KOI8-U" done for l in zh zh_CN; do #echo "$l GB_2312-80" # not a commonly used encoding, wrong encoding name echo "$l GB2312" done for l in ja ja_JP ja_JP.EUC; do echo "$l EUC-JP" done for l in ko ko_KR; do echo "$l EUC-KR" done for l in th th_TH; do echo "$l TIS-620" done for l in fa fa_IR; do #echo "$l ISIRI-3342" # a broken encoding echo "$l.utf-8 UTF-8" done ;; linux* | *-gnu*) # With glibc-2.1 or newer, we don't need any canonicalization, # because glibc has iconv and both glibc and libiconv support all # GNU canonical names directly. Therefore, the Makefile does not # need to install the alias file at all. # The following applies only to glibc-2.0.x and older libcs. echo "ISO_646.IRV:1983 ASCII" ;; aix*) echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-6 ISO-8859-6" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-8 ISO-8859-8" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-15 ISO-8859-15" echo "IBM-850 CP850" echo "IBM-856 CP856" echo "IBM-921 ISO-8859-13" echo "IBM-922 CP922" echo "IBM-932 CP932" echo "IBM-943 CP943" echo "IBM-1046 CP1046" echo "IBM-1124 CP1124" echo "IBM-1129 CP1129" echo "IBM-1252 CP1252" echo "IBM-eucCN GB2312" echo "IBM-eucJP EUC-JP" echo "IBM-eucKR EUC-KR" echo "IBM-eucTW EUC-TW" echo "big5 BIG5" echo "GBK GBK" echo "TIS-620 TIS-620" echo "UTF-8 UTF-8" ;; hpux*) echo "iso88591 ISO-8859-1" echo "iso88592 ISO-8859-2" echo "iso88595 ISO-8859-5" echo "iso88596 ISO-8859-6" echo "iso88597 ISO-8859-7" echo "iso88598 ISO-8859-8" echo "iso88599 ISO-8859-9" echo "iso885915 ISO-8859-15" echo "roman8 HP-ROMAN8" echo "arabic8 HP-ARABIC8" echo "greek8 HP-GREEK8" echo "hebrew8 HP-HEBREW8" echo "turkish8 HP-TURKISH8" echo "kana8 HP-KANA8" echo "tis620 TIS-620" echo "big5 BIG5" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" echo "hp15CN GB2312" #echo "ccdc ?" # what is this? echo "SJIS SHIFT_JIS" echo "utf8 UTF-8" ;; irix*) echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-9 ISO-8859-9" echo "eucCN GB2312" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" ;; osf*) echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-8 ISO-8859-8" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-15 ISO-8859-15" echo "cp850 CP850" echo "big5 BIG5" echo "dechanyu DEC-HANYU" echo "dechanzi GB2312" echo "deckanji DEC-KANJI" echo "deckorean EUC-KR" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" echo "GBK GBK" echo "KSC5601 CP949" echo "sdeckanji EUC-JP" echo "SJIS SHIFT_JIS" echo "TACTIS TIS-620" echo "UTF-8 UTF-8" ;; solaris*) echo "646 ASCII" echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-3 ISO-8859-3" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-6 ISO-8859-6" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-8 ISO-8859-8" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-15 ISO-8859-15" echo "koi8-r KOI8-R" echo "ansi-1251 CP1251" echo "BIG5 BIG5" echo "Big5-HKSCS BIG5-HKSCS" echo "gb2312 GB2312" echo "GBK GBK" echo "GB18030 GB18030" echo "cns11643 EUC-TW" echo "5601 EUC-KR" echo "ko_KR.johap92 JOHAB" echo "eucJP EUC-JP" echo "PCK SHIFT_JIS" echo "TIS620.2533 TIS-620" #echo "sun_eu_greek ?" # what is this? echo "UTF-8 UTF-8" ;; freebsd*) # FreeBSD 4.2 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "C ASCII" echo "US-ASCII ASCII" for l in la_LN lt_LN; do echo "$l.ASCII ASCII" done for l in da_DK de_AT de_CH de_DE en_AU en_CA en_GB en_US es_ES \ fi_FI fr_BE fr_CA fr_CH fr_FR is_IS it_CH it_IT la_LN \ lt_LN nl_BE nl_NL no_NO pt_PT sv_SE; do echo "$l.ISO_8859-1 ISO-8859-1" echo "$l.DIS_8859-15 ISO-8859-15" done for l in cs_CZ hr_HR hu_HU la_LN lt_LN pl_PL sl_SI; do echo "$l.ISO_8859-2 ISO-8859-2" done for l in la_LN lt_LT; do echo "$l.ISO_8859-4 ISO-8859-4" done for l in ru_RU ru_SU; do echo "$l.KOI8-R KOI8-R" echo "$l.ISO_8859-5 ISO-8859-5" echo "$l.CP866 CP866" done echo "uk_UA.KOI8-U KOI8-U" echo "zh_TW.BIG5 BIG5" echo "zh_TW.Big5 BIG5" echo "zh_CN.EUC GB2312" echo "ja_JP.EUC EUC-JP" echo "ja_JP.SJIS SHIFT_JIS" echo "ja_JP.Shift_JIS SHIFT_JIS" echo "ko_KR.EUC EUC-KR" ;; netbsd*) echo "646 ASCII" echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-13 ISO-8859-13" echo "ISO8859-15 ISO-8859-15" echo "eucCN GB2312" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "eucTW EUC-TW" echo "BIG5 BIG5" echo "SJIS SHIFT_JIS" ;; openbsd*) echo "646 ASCII" echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-13 ISO-8859-13" echo "ISO8859-15 ISO-8859-15" ;; darwin[56]*) # Darwin 6.8 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "C ASCII" for l in en_AU en_CA en_GB en_US la_LN; do echo "$l.US-ASCII ASCII" done for l in da_DK de_AT de_CH de_DE en_AU en_CA en_GB en_US es_ES \ fi_FI fr_BE fr_CA fr_CH fr_FR is_IS it_CH it_IT nl_BE \ nl_NL no_NO pt_PT sv_SE; do echo "$l ISO-8859-1" echo "$l.ISO8859-1 ISO-8859-1" echo "$l.ISO8859-15 ISO-8859-15" done for l in la_LN; do echo "$l.ISO8859-1 ISO-8859-1" echo "$l.ISO8859-15 ISO-8859-15" done for l in cs_CZ hr_HR hu_HU la_LN pl_PL sl_SI; do echo "$l.ISO8859-2 ISO-8859-2" done for l in la_LN lt_LT; do echo "$l.ISO8859-4 ISO-8859-4" done for l in ru_RU; do echo "$l.KOI8-R KOI8-R" echo "$l.ISO8859-5 ISO-8859-5" echo "$l.CP866 CP866" done for l in bg_BG; do echo "$l.CP1251 CP1251" done echo "uk_UA.KOI8-U KOI8-U" echo "zh_TW.BIG5 BIG5" echo "zh_TW.Big5 BIG5" echo "zh_CN.EUC GB2312" echo "ja_JP.EUC EUC-JP" echo "ja_JP.SJIS SHIFT_JIS" echo "ko_KR.EUC EUC-KR" ;; darwin*) # Darwin 7.5 has nl_langinfo(CODESET), but sometimes its value is # useless: # - It returns the empty string when LANG is set to a locale of the # form ll_CC, although ll_CC/LC_CTYPE is a symlink to an UTF-8 # LC_CTYPE file. # - The environment variables LANG, LC_CTYPE, LC_ALL are not set by # the system; nl_langinfo(CODESET) returns "US-ASCII" in this case. # - The documentation says: # "... all code that calls BSD system routines should ensure # that the const *char parameters of these routines are in UTF-8 # encoding. All BSD system functions expect their string # parameters to be in UTF-8 encoding and nothing else." # It also says # "An additional caveat is that string parameters for files, # paths, and other file-system entities must be in canonical # UTF-8. In a canonical UTF-8 Unicode string, all decomposable # characters are decomposed ..." # but this is not true: You can pass non-decomposed UTF-8 strings # to file system functions, and it is the OS which will convert # them to decomposed UTF-8 before accessing the file system. # - The Apple Terminal application displays UTF-8 by default. # - However, other applications are free to use different encodings: # - xterm uses ISO-8859-1 by default. # - TextEdit uses MacRoman by default. # We prefer UTF-8 over decomposed UTF-8-MAC because one should # minimize the use of decomposed Unicode. Unfortunately, through the # Darwin file system, decomposed UTF-8 strings are leaked into user # space nevertheless. # Then there are also the locales with encodings other than US-ASCII # and UTF-8. These locales can be occasionally useful to users (e.g. # when grepping through ISO-8859-1 encoded text files), when all their # file names are in US-ASCII. echo "ISO8859-1 ISO-8859-1" echo "ISO8859-2 ISO-8859-2" echo "ISO8859-4 ISO-8859-4" echo "ISO8859-5 ISO-8859-5" echo "ISO8859-7 ISO-8859-7" echo "ISO8859-9 ISO-8859-9" echo "ISO8859-13 ISO-8859-13" echo "ISO8859-15 ISO-8859-15" echo "KOI8-R KOI8-R" echo "KOI8-U KOI8-U" echo "CP866 CP866" echo "CP949 CP949" echo "CP1131 CP1131" echo "CP1251 CP1251" echo "eucCN GB2312" echo "GB2312 GB2312" echo "eucJP EUC-JP" echo "eucKR EUC-KR" echo "Big5 BIG5" echo "Big5HKSCS BIG5-HKSCS" echo "GBK GBK" echo "GB18030 GB18030" echo "SJIS SHIFT_JIS" echo "ARMSCII-8 ARMSCII-8" echo "PT154 PT154" #echo "ISCII-DEV ?" echo "* UTF-8" ;; beos* | haiku*) # BeOS and Haiku have a single locale, and it has UTF-8 encoding. echo "* UTF-8" ;; msdosdjgpp*) # DJGPP 2.03 doesn't have nl_langinfo(CODESET); therefore # localcharset.c falls back to using the full locale name # from the environment variables. echo "#" echo "# The encodings given here may not all be correct." echo "# If you find that the encoding given for your language and" echo "# country is not the one your DOS machine actually uses, just" echo "# correct it in this file, and send a mail to" echo "# Juan Manuel Guerrero " echo "# and Bruno Haible ." echo "#" echo "C ASCII" # ISO-8859-1 languages echo "ca CP850" echo "ca_ES CP850" echo "da CP865" # not CP850 ?? echo "da_DK CP865" # not CP850 ?? echo "de CP850" echo "de_AT CP850" echo "de_CH CP850" echo "de_DE CP850" echo "en CP850" echo "en_AU CP850" # not CP437 ?? echo "en_CA CP850" echo "en_GB CP850" echo "en_NZ CP437" echo "en_US CP437" echo "en_ZA CP850" # not CP437 ?? echo "es CP850" echo "es_AR CP850" echo "es_BO CP850" echo "es_CL CP850" echo "es_CO CP850" echo "es_CR CP850" echo "es_CU CP850" echo "es_DO CP850" echo "es_EC CP850" echo "es_ES CP850" echo "es_GT CP850" echo "es_HN CP850" echo "es_MX CP850" echo "es_NI CP850" echo "es_PA CP850" echo "es_PY CP850" echo "es_PE CP850" echo "es_SV CP850" echo "es_UY CP850" echo "es_VE CP850" echo "et CP850" echo "et_EE CP850" echo "eu CP850" echo "eu_ES CP850" echo "fi CP850" echo "fi_FI CP850" echo "fr CP850" echo "fr_BE CP850" echo "fr_CA CP850" echo "fr_CH CP850" echo "fr_FR CP850" echo "ga CP850" echo "ga_IE CP850" echo "gd CP850" echo "gd_GB CP850" echo "gl CP850" echo "gl_ES CP850" echo "id CP850" # not CP437 ?? echo "id_ID CP850" # not CP437 ?? echo "is CP861" # not CP850 ?? echo "is_IS CP861" # not CP850 ?? echo "it CP850" echo "it_CH CP850" echo "it_IT CP850" echo "lt CP775" echo "lt_LT CP775" echo "lv CP775" echo "lv_LV CP775" echo "nb CP865" # not CP850 ?? echo "nb_NO CP865" # not CP850 ?? echo "nl CP850" echo "nl_BE CP850" echo "nl_NL CP850" echo "nn CP865" # not CP850 ?? echo "nn_NO CP865" # not CP850 ?? echo "no CP865" # not CP850 ?? echo "no_NO CP865" # not CP850 ?? echo "pt CP850" echo "pt_BR CP850" echo "pt_PT CP850" echo "sv CP850" echo "sv_SE CP850" # ISO-8859-2 languages echo "cs CP852" echo "cs_CZ CP852" echo "hr CP852" echo "hr_HR CP852" echo "hu CP852" echo "hu_HU CP852" echo "pl CP852" echo "pl_PL CP852" echo "ro CP852" echo "ro_RO CP852" echo "sk CP852" echo "sk_SK CP852" echo "sl CP852" echo "sl_SI CP852" echo "sq CP852" echo "sq_AL CP852" echo "sr CP852" # CP852 or CP866 or CP855 ?? echo "sr_CS CP852" # CP852 or CP866 or CP855 ?? echo "sr_YU CP852" # CP852 or CP866 or CP855 ?? # ISO-8859-3 languages echo "mt CP850" echo "mt_MT CP850" # ISO-8859-5 languages echo "be CP866" echo "be_BE CP866" echo "bg CP866" # not CP855 ?? echo "bg_BG CP866" # not CP855 ?? echo "mk CP866" # not CP855 ?? echo "mk_MK CP866" # not CP855 ?? echo "ru CP866" echo "ru_RU CP866" echo "uk CP1125" echo "uk_UA CP1125" # ISO-8859-6 languages echo "ar CP864" echo "ar_AE CP864" echo "ar_DZ CP864" echo "ar_EG CP864" echo "ar_IQ CP864" echo "ar_IR CP864" echo "ar_JO CP864" echo "ar_KW CP864" echo "ar_MA CP864" echo "ar_OM CP864" echo "ar_QA CP864" echo "ar_SA CP864" echo "ar_SY CP864" # ISO-8859-7 languages echo "el CP869" echo "el_GR CP869" # ISO-8859-8 languages echo "he CP862" echo "he_IL CP862" # ISO-8859-9 languages echo "tr CP857" echo "tr_TR CP857" # Japanese echo "ja CP932" echo "ja_JP CP932" # Chinese echo "zh_CN GBK" echo "zh_TW CP950" # not CP938 ?? # Korean echo "kr CP949" # not CP934 ?? echo "kr_KR CP949" # not CP934 ?? # Thai echo "th CP874" echo "th_TH CP874" # Other echo "eo CP850" echo "eo_EO CP850" ;; esac gnuastro-0.5/bootstrapped/lib/limits.in.h0000644000175000017500000000605113217200021015462 00000000000000/* A GNU-like . Copyright 2016-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_LIMITS_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_LIMITS_H@ #ifndef _@GUARD_PREFIX@_LIMITS_H #define _@GUARD_PREFIX@_LIMITS_H /* For HP-UX 11.31. */ #if defined LONG_LONG_MIN && !defined LLONG_MIN # define LLONG_MIN LONG_LONG_MIN #endif #if defined LONG_LONG_MAX && !defined LLONG_MAX # define LLONG_MAX LONG_LONG_MAX #endif #if defined ULONG_LONG_MAX && !defined ULLONG_MAX # define ULLONG_MAX ULONG_LONG_MAX #endif /* The number of usable bits in an unsigned or signed integer type with minimum value MIN and maximum value MAX, as an int expression suitable in #if. Cover all known practical hosts. This implementation exploits the fact that MAX is 1 less than a power of 2, and merely counts the number of 1 bits in MAX; "COBn" means "count the number of 1 bits in the low-order n bits"). */ #define _GL_INTEGER_WIDTH(min, max) (((min) < 0) + _GL_COB128 (max)) #define _GL_COB128(n) (_GL_COB64 ((n) >> 31 >> 31 >> 2) + _GL_COB64 (n)) #define _GL_COB64(n) (_GL_COB32 ((n) >> 31 >> 1) + _GL_COB32 (n)) #define _GL_COB32(n) (_GL_COB16 ((n) >> 16) + _GL_COB16 (n)) #define _GL_COB16(n) (_GL_COB8 ((n) >> 8) + _GL_COB8 (n)) #define _GL_COB8(n) (_GL_COB4 ((n) >> 4) + _GL_COB4 (n)) #define _GL_COB4(n) (!!((n) & 8) + !!((n) & 4) + !!((n) & 2) + !!((n) & 1)) /* Macros specified by ISO/IEC TS 18661-1:2014. */ #if (! defined ULLONG_WIDTH \ && (defined _GNU_SOURCE || defined __STDC_WANT_IEC_60559_BFP_EXT__)) # define CHAR_WIDTH _GL_INTEGER_WIDTH (CHAR_MIN, CHAR_MAX) # define SCHAR_WIDTH _GL_INTEGER_WIDTH (SCHAR_MIN, SCHAR_MAX) # define UCHAR_WIDTH _GL_INTEGER_WIDTH (0, UCHAR_MAX) # define SHRT_WIDTH _GL_INTEGER_WIDTH (SHRT_MIN, SHRT_MAX) # define USHRT_WIDTH _GL_INTEGER_WIDTH (0, USHRT_MAX) # define INT_WIDTH _GL_INTEGER_WIDTH (INT_MIN, INT_MAX) # define UINT_WIDTH _GL_INTEGER_WIDTH (0, UINT_MAX) # define LONG_WIDTH _GL_INTEGER_WIDTH (LONG_MIN, LONG_MAX) # define ULONG_WIDTH _GL_INTEGER_WIDTH (0, ULONG_MAX) # define LLONG_WIDTH _GL_INTEGER_WIDTH (LLONG_MIN, LLONG_MAX) # define ULLONG_WIDTH _GL_INTEGER_WIDTH (0, ULLONG_MAX) #endif /* !ULLONG_WIDTH && (_GNU_SOURCE || __STDC_WANT_IEC_60559_BFP_EXT__) */ #endif /* _@GUARD_PREFIX@_LIMITS_H */ #endif /* _@GUARD_PREFIX@_LIMITS_H */ gnuastro-0.5/bootstrapped/lib/langinfo.in.h0000644000175000017500000001321313217200021015754 00000000000000/* Substitute for and wrapper around . Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* * POSIX for platforms that lack it or have an incomplete one. * */ #ifndef _@GUARD_PREFIX@_LANGINFO_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #if @HAVE_LANGINFO_H@ # @INCLUDE_NEXT@ @NEXT_LANGINFO_H@ #endif #ifndef _@GUARD_PREFIX@_LANGINFO_H #define _@GUARD_PREFIX@_LANGINFO_H #if !@HAVE_LANGINFO_H@ /* A platform that lacks . */ /* Assume that it also lacks and the nl_item type. */ # if !GNULIB_defined_nl_item typedef int nl_item; # define GNULIB_defined_nl_item 1 # endif /* nl_langinfo items of the LC_CTYPE category */ # define CODESET 10000 /* nl_langinfo items of the LC_NUMERIC category */ # define RADIXCHAR 10001 # define DECIMAL_POINT RADIXCHAR # define THOUSEP 10002 # define THOUSANDS_SEP THOUSEP # define GROUPING 10114 /* nl_langinfo items of the LC_TIME category */ # define D_T_FMT 10003 # define D_FMT 10004 # define T_FMT 10005 # define T_FMT_AMPM 10006 # define AM_STR 10007 # define PM_STR 10008 # define DAY_1 10009 # define DAY_2 (DAY_1 + 1) # define DAY_3 (DAY_1 + 2) # define DAY_4 (DAY_1 + 3) # define DAY_5 (DAY_1 + 4) # define DAY_6 (DAY_1 + 5) # define DAY_7 (DAY_1 + 6) # define ABDAY_1 10016 # define ABDAY_2 (ABDAY_1 + 1) # define ABDAY_3 (ABDAY_1 + 2) # define ABDAY_4 (ABDAY_1 + 3) # define ABDAY_5 (ABDAY_1 + 4) # define ABDAY_6 (ABDAY_1 + 5) # define ABDAY_7 (ABDAY_1 + 6) # define MON_1 10023 # define MON_2 (MON_1 + 1) # define MON_3 (MON_1 + 2) # define MON_4 (MON_1 + 3) # define MON_5 (MON_1 + 4) # define MON_6 (MON_1 + 5) # define MON_7 (MON_1 + 6) # define MON_8 (MON_1 + 7) # define MON_9 (MON_1 + 8) # define MON_10 (MON_1 + 9) # define MON_11 (MON_1 + 10) # define MON_12 (MON_1 + 11) # define ABMON_1 10035 # define ABMON_2 (ABMON_1 + 1) # define ABMON_3 (ABMON_1 + 2) # define ABMON_4 (ABMON_1 + 3) # define ABMON_5 (ABMON_1 + 4) # define ABMON_6 (ABMON_1 + 5) # define ABMON_7 (ABMON_1 + 6) # define ABMON_8 (ABMON_1 + 7) # define ABMON_9 (ABMON_1 + 8) # define ABMON_10 (ABMON_1 + 9) # define ABMON_11 (ABMON_1 + 10) # define ABMON_12 (ABMON_1 + 11) # define ERA 10047 # define ERA_D_FMT 10048 # define ERA_D_T_FMT 10049 # define ERA_T_FMT 10050 # define ALT_DIGITS 10051 /* nl_langinfo items of the LC_MONETARY category */ # define CRNCYSTR 10052 # define CURRENCY_SYMBOL CRNCYSTR # define INT_CURR_SYMBOL 10100 # define MON_DECIMAL_POINT 10101 # define MON_THOUSANDS_SEP 10102 # define MON_GROUPING 10103 # define POSITIVE_SIGN 10104 # define NEGATIVE_SIGN 10105 # define FRAC_DIGITS 10106 # define INT_FRAC_DIGITS 10107 # define P_CS_PRECEDES 10108 # define N_CS_PRECEDES 10109 # define P_SEP_BY_SPACE 10110 # define N_SEP_BY_SPACE 10111 # define P_SIGN_POSN 10112 # define N_SIGN_POSN 10113 /* nl_langinfo items of the LC_MESSAGES category */ # define YESEXPR 10053 # define NOEXPR 10054 #else /* A platform that has . */ # if !@HAVE_LANGINFO_CODESET@ # define CODESET 10000 # define GNULIB_defined_CODESET 1 # endif # if !@HAVE_LANGINFO_T_FMT_AMPM@ # define T_FMT_AMPM 10006 # define GNULIB_defined_T_FMT_AMPM 1 # endif # if !@HAVE_LANGINFO_ERA@ # define ERA 10047 # define ERA_D_FMT 10048 # define ERA_D_T_FMT 10049 # define ERA_T_FMT 10050 # define ALT_DIGITS 10051 # define GNULIB_defined_ERA 1 # endif # if !@HAVE_LANGINFO_YESEXPR@ # define YESEXPR 10053 # define NOEXPR 10054 # define GNULIB_defined_YESEXPR 1 # endif #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* Declare overridden functions. */ /* Return a piece of locale dependent information. Note: The difference between nl_langinfo (CODESET) and locale_charset () is that the latter normalizes the encoding names to GNU conventions. */ #if @GNULIB_NL_LANGINFO@ # if @REPLACE_NL_LANGINFO@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef nl_langinfo # define nl_langinfo rpl_nl_langinfo # endif _GL_FUNCDECL_RPL (nl_langinfo, char *, (nl_item item)); _GL_CXXALIAS_RPL (nl_langinfo, char *, (nl_item item)); # else # if !@HAVE_NL_LANGINFO@ _GL_FUNCDECL_SYS (nl_langinfo, char *, (nl_item item)); # endif _GL_CXXALIAS_SYS (nl_langinfo, char *, (nl_item item)); # endif _GL_CXXALIASWARN (nl_langinfo); #elif defined GNULIB_POSIXCHECK # undef nl_langinfo # if HAVE_RAW_DECL_NL_LANGINFO _GL_WARN_ON_USE (nl_langinfo, "nl_langinfo is not portable - " "use gnulib module nl_langinfo for portability"); # endif #endif #endif /* _@GUARD_PREFIX@_LANGINFO_H */ #endif /* _@GUARD_PREFIX@_LANGINFO_H */ gnuastro-0.5/bootstrapped/lib/inttypes.in.h0000644000175000017500000006476213217200021016055 00000000000000/* Copyright (C) 2006-2017 Free Software Foundation, Inc. Written by Paul Eggert, Bruno Haible, Derek Price. This file is part of gnulib. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* * ISO C 99 for platforms that lack it. * */ #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* Include the original if it exists, and if this file has not been included yet or if this file includes gnulib stdint.h which in turn includes this file. The include_next requires a split double-inclusion guard. */ #if ! defined INTTYPES_H || defined _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H # if @HAVE_INTTYPES_H@ /* Some pre-C++11 implementations need this. */ # if defined __cplusplus && ! defined __STDC_FORMAT_MACROS # define __STDC_FORMAT_MACROS 1 # endif # @INCLUDE_NEXT@ @NEXT_INTTYPES_H@ # endif #endif #if ! defined INTTYPES_H && ! defined _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H #define INTTYPES_H /* Include or the gnulib replacement. But avoid namespace pollution on glibc systems. */ #ifndef __GLIBC__ # include #endif /* Get CHAR_BIT. */ #include /* On mingw, __USE_MINGW_ANSI_STDIO only works if is also included */ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include #endif #if !(INT_MIN == INT32_MIN && INT_MAX == INT32_MAX) # error "This file assumes that 'int' has exactly 32 bits. Please report your platform and compiler to ." #endif /* The definitions of _GL_FUNCDECL_RPL etc. are copied here. */ /* The definition of _GL_ARG_NONNULL is copied here. */ /* The definition of _GL_WARN_ON_USE is copied here. */ /* 7.8.1 Macros for format specifiers */ #if defined _TNS_R_TARGET /* Tandem NonStop R series and compatible platforms released before July 2005 support %Ld but not %lld. */ # define _LONG_LONG_FORMAT_PREFIX "L" #else # define _LONG_LONG_FORMAT_PREFIX "ll" #endif #if !defined PRId8 || @PRI_MACROS_BROKEN@ # undef PRId8 # ifdef INT8_MAX # define PRId8 "d" # endif #endif #if !defined PRIi8 || @PRI_MACROS_BROKEN@ # undef PRIi8 # ifdef INT8_MAX # define PRIi8 "i" # endif #endif #if !defined PRIo8 || @PRI_MACROS_BROKEN@ # undef PRIo8 # ifdef UINT8_MAX # define PRIo8 "o" # endif #endif #if !defined PRIu8 || @PRI_MACROS_BROKEN@ # undef PRIu8 # ifdef UINT8_MAX # define PRIu8 "u" # endif #endif #if !defined PRIx8 || @PRI_MACROS_BROKEN@ # undef PRIx8 # ifdef UINT8_MAX # define PRIx8 "x" # endif #endif #if !defined PRIX8 || @PRI_MACROS_BROKEN@ # undef PRIX8 # ifdef UINT8_MAX # define PRIX8 "X" # endif #endif #if !defined PRId16 || @PRI_MACROS_BROKEN@ # undef PRId16 # ifdef INT16_MAX # define PRId16 "d" # endif #endif #if !defined PRIi16 || @PRI_MACROS_BROKEN@ # undef PRIi16 # ifdef INT16_MAX # define PRIi16 "i" # endif #endif #if !defined PRIo16 || @PRI_MACROS_BROKEN@ # undef PRIo16 # ifdef UINT16_MAX # define PRIo16 "o" # endif #endif #if !defined PRIu16 || @PRI_MACROS_BROKEN@ # undef PRIu16 # ifdef UINT16_MAX # define PRIu16 "u" # endif #endif #if !defined PRIx16 || @PRI_MACROS_BROKEN@ # undef PRIx16 # ifdef UINT16_MAX # define PRIx16 "x" # endif #endif #if !defined PRIX16 || @PRI_MACROS_BROKEN@ # undef PRIX16 # ifdef UINT16_MAX # define PRIX16 "X" # endif #endif #if !defined PRId32 || @PRI_MACROS_BROKEN@ # undef PRId32 # ifdef INT32_MAX # define PRId32 "d" # endif #endif #if !defined PRIi32 || @PRI_MACROS_BROKEN@ # undef PRIi32 # ifdef INT32_MAX # define PRIi32 "i" # endif #endif #if !defined PRIo32 || @PRI_MACROS_BROKEN@ # undef PRIo32 # ifdef UINT32_MAX # define PRIo32 "o" # endif #endif #if !defined PRIu32 || @PRI_MACROS_BROKEN@ # undef PRIu32 # ifdef UINT32_MAX # define PRIu32 "u" # endif #endif #if !defined PRIx32 || @PRI_MACROS_BROKEN@ # undef PRIx32 # ifdef UINT32_MAX # define PRIx32 "x" # endif #endif #if !defined PRIX32 || @PRI_MACROS_BROKEN@ # undef PRIX32 # ifdef UINT32_MAX # define PRIX32 "X" # endif #endif #ifdef INT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @INT64_MAX_EQ_LONG_MAX@) # define _PRI64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _PRI64_PREFIX "I64" # elif @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 # define _PRI64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined PRId64 || @PRI_MACROS_BROKEN@ # undef PRId64 # define PRId64 _PRI64_PREFIX "d" # endif # if !defined PRIi64 || @PRI_MACROS_BROKEN@ # undef PRIi64 # define PRIi64 _PRI64_PREFIX "i" # endif #endif #ifdef UINT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @UINT64_MAX_EQ_ULONG_MAX@) # define _PRIu64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _PRIu64_PREFIX "I64" # elif @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 # define _PRIu64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined PRIo64 || @PRI_MACROS_BROKEN@ # undef PRIo64 # define PRIo64 _PRIu64_PREFIX "o" # endif # if !defined PRIu64 || @PRI_MACROS_BROKEN@ # undef PRIu64 # define PRIu64 _PRIu64_PREFIX "u" # endif # if !defined PRIx64 || @PRI_MACROS_BROKEN@ # undef PRIx64 # define PRIx64 _PRIu64_PREFIX "x" # endif # if !defined PRIX64 || @PRI_MACROS_BROKEN@ # undef PRIX64 # define PRIX64 _PRIu64_PREFIX "X" # endif #endif #if !defined PRIdLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST8 # define PRIdLEAST8 "d" #endif #if !defined PRIiLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST8 # define PRIiLEAST8 "i" #endif #if !defined PRIoLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST8 # define PRIoLEAST8 "o" #endif #if !defined PRIuLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST8 # define PRIuLEAST8 "u" #endif #if !defined PRIxLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST8 # define PRIxLEAST8 "x" #endif #if !defined PRIXLEAST8 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST8 # define PRIXLEAST8 "X" #endif #if !defined PRIdLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST16 # define PRIdLEAST16 "d" #endif #if !defined PRIiLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST16 # define PRIiLEAST16 "i" #endif #if !defined PRIoLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST16 # define PRIoLEAST16 "o" #endif #if !defined PRIuLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST16 # define PRIuLEAST16 "u" #endif #if !defined PRIxLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST16 # define PRIxLEAST16 "x" #endif #if !defined PRIXLEAST16 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST16 # define PRIXLEAST16 "X" #endif #if !defined PRIdLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST32 # define PRIdLEAST32 "d" #endif #if !defined PRIiLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST32 # define PRIiLEAST32 "i" #endif #if !defined PRIoLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST32 # define PRIoLEAST32 "o" #endif #if !defined PRIuLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST32 # define PRIuLEAST32 "u" #endif #if !defined PRIxLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST32 # define PRIxLEAST32 "x" #endif #if !defined PRIXLEAST32 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST32 # define PRIXLEAST32 "X" #endif #ifdef INT64_MAX # if !defined PRIdLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIdLEAST64 # define PRIdLEAST64 PRId64 # endif # if !defined PRIiLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIiLEAST64 # define PRIiLEAST64 PRIi64 # endif #endif #ifdef UINT64_MAX # if !defined PRIoLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIoLEAST64 # define PRIoLEAST64 PRIo64 # endif # if !defined PRIuLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIuLEAST64 # define PRIuLEAST64 PRIu64 # endif # if !defined PRIxLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIxLEAST64 # define PRIxLEAST64 PRIx64 # endif # if !defined PRIXLEAST64 || @PRI_MACROS_BROKEN@ # undef PRIXLEAST64 # define PRIXLEAST64 PRIX64 # endif #endif #if !defined PRIdFAST8 || @PRI_MACROS_BROKEN@ # undef PRIdFAST8 # if INT_FAST8_MAX > INT32_MAX # define PRIdFAST8 PRId64 # else # define PRIdFAST8 "d" # endif #endif #if !defined PRIiFAST8 || @PRI_MACROS_BROKEN@ # undef PRIiFAST8 # if INT_FAST8_MAX > INT32_MAX # define PRIiFAST8 PRIi64 # else # define PRIiFAST8 "i" # endif #endif #if !defined PRIoFAST8 || @PRI_MACROS_BROKEN@ # undef PRIoFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIoFAST8 PRIo64 # else # define PRIoFAST8 "o" # endif #endif #if !defined PRIuFAST8 || @PRI_MACROS_BROKEN@ # undef PRIuFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIuFAST8 PRIu64 # else # define PRIuFAST8 "u" # endif #endif #if !defined PRIxFAST8 || @PRI_MACROS_BROKEN@ # undef PRIxFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIxFAST8 PRIx64 # else # define PRIxFAST8 "x" # endif #endif #if !defined PRIXFAST8 || @PRI_MACROS_BROKEN@ # undef PRIXFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define PRIXFAST8 PRIX64 # else # define PRIXFAST8 "X" # endif #endif #if !defined PRIdFAST16 || @PRI_MACROS_BROKEN@ # undef PRIdFAST16 # if INT_FAST16_MAX > INT32_MAX # define PRIdFAST16 PRId64 # else # define PRIdFAST16 "d" # endif #endif #if !defined PRIiFAST16 || @PRI_MACROS_BROKEN@ # undef PRIiFAST16 # if INT_FAST16_MAX > INT32_MAX # define PRIiFAST16 PRIi64 # else # define PRIiFAST16 "i" # endif #endif #if !defined PRIoFAST16 || @PRI_MACROS_BROKEN@ # undef PRIoFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIoFAST16 PRIo64 # else # define PRIoFAST16 "o" # endif #endif #if !defined PRIuFAST16 || @PRI_MACROS_BROKEN@ # undef PRIuFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIuFAST16 PRIu64 # else # define PRIuFAST16 "u" # endif #endif #if !defined PRIxFAST16 || @PRI_MACROS_BROKEN@ # undef PRIxFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIxFAST16 PRIx64 # else # define PRIxFAST16 "x" # endif #endif #if !defined PRIXFAST16 || @PRI_MACROS_BROKEN@ # undef PRIXFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define PRIXFAST16 PRIX64 # else # define PRIXFAST16 "X" # endif #endif #if !defined PRIdFAST32 || @PRI_MACROS_BROKEN@ # undef PRIdFAST32 # if INT_FAST32_MAX > INT32_MAX # define PRIdFAST32 PRId64 # else # define PRIdFAST32 "d" # endif #endif #if !defined PRIiFAST32 || @PRI_MACROS_BROKEN@ # undef PRIiFAST32 # if INT_FAST32_MAX > INT32_MAX # define PRIiFAST32 PRIi64 # else # define PRIiFAST32 "i" # endif #endif #if !defined PRIoFAST32 || @PRI_MACROS_BROKEN@ # undef PRIoFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIoFAST32 PRIo64 # else # define PRIoFAST32 "o" # endif #endif #if !defined PRIuFAST32 || @PRI_MACROS_BROKEN@ # undef PRIuFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIuFAST32 PRIu64 # else # define PRIuFAST32 "u" # endif #endif #if !defined PRIxFAST32 || @PRI_MACROS_BROKEN@ # undef PRIxFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIxFAST32 PRIx64 # else # define PRIxFAST32 "x" # endif #endif #if !defined PRIXFAST32 || @PRI_MACROS_BROKEN@ # undef PRIXFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define PRIXFAST32 PRIX64 # else # define PRIXFAST32 "X" # endif #endif #ifdef INT64_MAX # if !defined PRIdFAST64 || @PRI_MACROS_BROKEN@ # undef PRIdFAST64 # define PRIdFAST64 PRId64 # endif # if !defined PRIiFAST64 || @PRI_MACROS_BROKEN@ # undef PRIiFAST64 # define PRIiFAST64 PRIi64 # endif #endif #ifdef UINT64_MAX # if !defined PRIoFAST64 || @PRI_MACROS_BROKEN@ # undef PRIoFAST64 # define PRIoFAST64 PRIo64 # endif # if !defined PRIuFAST64 || @PRI_MACROS_BROKEN@ # undef PRIuFAST64 # define PRIuFAST64 PRIu64 # endif # if !defined PRIxFAST64 || @PRI_MACROS_BROKEN@ # undef PRIxFAST64 # define PRIxFAST64 PRIx64 # endif # if !defined PRIXFAST64 || @PRI_MACROS_BROKEN@ # undef PRIXFAST64 # define PRIXFAST64 PRIX64 # endif #endif #if !defined PRIdMAX || @PRI_MACROS_BROKEN@ # undef PRIdMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define PRIdMAX PRId64 # else # define PRIdMAX "ld" # endif #endif #if !defined PRIiMAX || @PRI_MACROS_BROKEN@ # undef PRIiMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define PRIiMAX PRIi64 # else # define PRIiMAX "li" # endif #endif #if !defined PRIoMAX || @PRI_MACROS_BROKEN@ # undef PRIoMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIoMAX PRIo64 # else # define PRIoMAX "lo" # endif #endif #if !defined PRIuMAX || @PRI_MACROS_BROKEN@ # undef PRIuMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIuMAX PRIu64 # else # define PRIuMAX "lu" # endif #endif #if !defined PRIxMAX || @PRI_MACROS_BROKEN@ # undef PRIxMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIxMAX PRIx64 # else # define PRIxMAX "lx" # endif #endif #if !defined PRIXMAX || @PRI_MACROS_BROKEN@ # undef PRIXMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define PRIXMAX PRIX64 # else # define PRIXMAX "lX" # endif #endif #if !defined PRIdPTR || @PRI_MACROS_BROKEN@ # undef PRIdPTR # ifdef INTPTR_MAX # define PRIdPTR @PRIPTR_PREFIX@ "d" # endif #endif #if !defined PRIiPTR || @PRI_MACROS_BROKEN@ # undef PRIiPTR # ifdef INTPTR_MAX # define PRIiPTR @PRIPTR_PREFIX@ "i" # endif #endif #if !defined PRIoPTR || @PRI_MACROS_BROKEN@ # undef PRIoPTR # ifdef UINTPTR_MAX # define PRIoPTR @PRIPTR_PREFIX@ "o" # endif #endif #if !defined PRIuPTR || @PRI_MACROS_BROKEN@ # undef PRIuPTR # ifdef UINTPTR_MAX # define PRIuPTR @PRIPTR_PREFIX@ "u" # endif #endif #if !defined PRIxPTR || @PRI_MACROS_BROKEN@ # undef PRIxPTR # ifdef UINTPTR_MAX # define PRIxPTR @PRIPTR_PREFIX@ "x" # endif #endif #if !defined PRIXPTR || @PRI_MACROS_BROKEN@ # undef PRIXPTR # ifdef UINTPTR_MAX # define PRIXPTR @PRIPTR_PREFIX@ "X" # endif #endif #if !defined SCNd8 || @PRI_MACROS_BROKEN@ # undef SCNd8 # ifdef INT8_MAX # define SCNd8 "hhd" # endif #endif #if !defined SCNi8 || @PRI_MACROS_BROKEN@ # undef SCNi8 # ifdef INT8_MAX # define SCNi8 "hhi" # endif #endif #if !defined SCNo8 || @PRI_MACROS_BROKEN@ # undef SCNo8 # ifdef UINT8_MAX # define SCNo8 "hho" # endif #endif #if !defined SCNu8 || @PRI_MACROS_BROKEN@ # undef SCNu8 # ifdef UINT8_MAX # define SCNu8 "hhu" # endif #endif #if !defined SCNx8 || @PRI_MACROS_BROKEN@ # undef SCNx8 # ifdef UINT8_MAX # define SCNx8 "hhx" # endif #endif #if !defined SCNd16 || @PRI_MACROS_BROKEN@ # undef SCNd16 # ifdef INT16_MAX # define SCNd16 "hd" # endif #endif #if !defined SCNi16 || @PRI_MACROS_BROKEN@ # undef SCNi16 # ifdef INT16_MAX # define SCNi16 "hi" # endif #endif #if !defined SCNo16 || @PRI_MACROS_BROKEN@ # undef SCNo16 # ifdef UINT16_MAX # define SCNo16 "ho" # endif #endif #if !defined SCNu16 || @PRI_MACROS_BROKEN@ # undef SCNu16 # ifdef UINT16_MAX # define SCNu16 "hu" # endif #endif #if !defined SCNx16 || @PRI_MACROS_BROKEN@ # undef SCNx16 # ifdef UINT16_MAX # define SCNx16 "hx" # endif #endif #if !defined SCNd32 || @PRI_MACROS_BROKEN@ # undef SCNd32 # ifdef INT32_MAX # define SCNd32 "d" # endif #endif #if !defined SCNi32 || @PRI_MACROS_BROKEN@ # undef SCNi32 # ifdef INT32_MAX # define SCNi32 "i" # endif #endif #if !defined SCNo32 || @PRI_MACROS_BROKEN@ # undef SCNo32 # ifdef UINT32_MAX # define SCNo32 "o" # endif #endif #if !defined SCNu32 || @PRI_MACROS_BROKEN@ # undef SCNu32 # ifdef UINT32_MAX # define SCNu32 "u" # endif #endif #if !defined SCNx32 || @PRI_MACROS_BROKEN@ # undef SCNx32 # ifdef UINT32_MAX # define SCNx32 "x" # endif #endif #ifdef INT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @INT64_MAX_EQ_LONG_MAX@) # define _SCN64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _SCN64_PREFIX "I64" # elif @HAVE_LONG_LONG_INT@ && LONG_MAX >> 30 == 1 # define _SCN64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined SCNd64 || @PRI_MACROS_BROKEN@ # undef SCNd64 # define SCNd64 _SCN64_PREFIX "d" # endif # if !defined SCNi64 || @PRI_MACROS_BROKEN@ # undef SCNi64 # define SCNi64 _SCN64_PREFIX "i" # endif #endif #ifdef UINT64_MAX # if (@APPLE_UNIVERSAL_BUILD@ ? defined _LP64 : @UINT64_MAX_EQ_ULONG_MAX@) # define _SCNu64_PREFIX "l" # elif defined _MSC_VER || defined __MINGW32__ # define _SCNu64_PREFIX "I64" # elif @HAVE_UNSIGNED_LONG_LONG_INT@ && ULONG_MAX >> 31 == 1 # define _SCNu64_PREFIX _LONG_LONG_FORMAT_PREFIX # endif # if !defined SCNo64 || @PRI_MACROS_BROKEN@ # undef SCNo64 # define SCNo64 _SCNu64_PREFIX "o" # endif # if !defined SCNu64 || @PRI_MACROS_BROKEN@ # undef SCNu64 # define SCNu64 _SCNu64_PREFIX "u" # endif # if !defined SCNx64 || @PRI_MACROS_BROKEN@ # undef SCNx64 # define SCNx64 _SCNu64_PREFIX "x" # endif #endif #if !defined SCNdLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST8 # define SCNdLEAST8 "hhd" #endif #if !defined SCNiLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST8 # define SCNiLEAST8 "hhi" #endif #if !defined SCNoLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST8 # define SCNoLEAST8 "hho" #endif #if !defined SCNuLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST8 # define SCNuLEAST8 "hhu" #endif #if !defined SCNxLEAST8 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST8 # define SCNxLEAST8 "hhx" #endif #if !defined SCNdLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST16 # define SCNdLEAST16 "hd" #endif #if !defined SCNiLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST16 # define SCNiLEAST16 "hi" #endif #if !defined SCNoLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST16 # define SCNoLEAST16 "ho" #endif #if !defined SCNuLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST16 # define SCNuLEAST16 "hu" #endif #if !defined SCNxLEAST16 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST16 # define SCNxLEAST16 "hx" #endif #if !defined SCNdLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST32 # define SCNdLEAST32 "d" #endif #if !defined SCNiLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST32 # define SCNiLEAST32 "i" #endif #if !defined SCNoLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST32 # define SCNoLEAST32 "o" #endif #if !defined SCNuLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST32 # define SCNuLEAST32 "u" #endif #if !defined SCNxLEAST32 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST32 # define SCNxLEAST32 "x" #endif #ifdef INT64_MAX # if !defined SCNdLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNdLEAST64 # define SCNdLEAST64 SCNd64 # endif # if !defined SCNiLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNiLEAST64 # define SCNiLEAST64 SCNi64 # endif #endif #ifdef UINT64_MAX # if !defined SCNoLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNoLEAST64 # define SCNoLEAST64 SCNo64 # endif # if !defined SCNuLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNuLEAST64 # define SCNuLEAST64 SCNu64 # endif # if !defined SCNxLEAST64 || @PRI_MACROS_BROKEN@ # undef SCNxLEAST64 # define SCNxLEAST64 SCNx64 # endif #endif #if !defined SCNdFAST8 || @PRI_MACROS_BROKEN@ # undef SCNdFAST8 # if INT_FAST8_MAX > INT32_MAX # define SCNdFAST8 SCNd64 # elif INT_FAST8_MAX == 0x7fff # define SCNdFAST8 "hd" # elif INT_FAST8_MAX == 0x7f # define SCNdFAST8 "hhd" # else # define SCNdFAST8 "d" # endif #endif #if !defined SCNiFAST8 || @PRI_MACROS_BROKEN@ # undef SCNiFAST8 # if INT_FAST8_MAX > INT32_MAX # define SCNiFAST8 SCNi64 # elif INT_FAST8_MAX == 0x7fff # define SCNiFAST8 "hi" # elif INT_FAST8_MAX == 0x7f # define SCNiFAST8 "hhi" # else # define SCNiFAST8 "i" # endif #endif #if !defined SCNoFAST8 || @PRI_MACROS_BROKEN@ # undef SCNoFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define SCNoFAST8 SCNo64 # elif UINT_FAST8_MAX == 0xffff # define SCNoFAST8 "ho" # elif UINT_FAST8_MAX == 0xff # define SCNoFAST8 "hho" # else # define SCNoFAST8 "o" # endif #endif #if !defined SCNuFAST8 || @PRI_MACROS_BROKEN@ # undef SCNuFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define SCNuFAST8 SCNu64 # elif UINT_FAST8_MAX == 0xffff # define SCNuFAST8 "hu" # elif UINT_FAST8_MAX == 0xff # define SCNuFAST8 "hhu" # else # define SCNuFAST8 "u" # endif #endif #if !defined SCNxFAST8 || @PRI_MACROS_BROKEN@ # undef SCNxFAST8 # if UINT_FAST8_MAX > UINT32_MAX # define SCNxFAST8 SCNx64 # elif UINT_FAST8_MAX == 0xffff # define SCNxFAST8 "hx" # elif UINT_FAST8_MAX == 0xff # define SCNxFAST8 "hhx" # else # define SCNxFAST8 "x" # endif #endif #if !defined SCNdFAST16 || @PRI_MACROS_BROKEN@ # undef SCNdFAST16 # if INT_FAST16_MAX > INT32_MAX # define SCNdFAST16 SCNd64 # elif INT_FAST16_MAX == 0x7fff # define SCNdFAST16 "hd" # else # define SCNdFAST16 "d" # endif #endif #if !defined SCNiFAST16 || @PRI_MACROS_BROKEN@ # undef SCNiFAST16 # if INT_FAST16_MAX > INT32_MAX # define SCNiFAST16 SCNi64 # elif INT_FAST16_MAX == 0x7fff # define SCNiFAST16 "hi" # else # define SCNiFAST16 "i" # endif #endif #if !defined SCNoFAST16 || @PRI_MACROS_BROKEN@ # undef SCNoFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define SCNoFAST16 SCNo64 # elif UINT_FAST16_MAX == 0xffff # define SCNoFAST16 "ho" # else # define SCNoFAST16 "o" # endif #endif #if !defined SCNuFAST16 || @PRI_MACROS_BROKEN@ # undef SCNuFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define SCNuFAST16 SCNu64 # elif UINT_FAST16_MAX == 0xffff # define SCNuFAST16 "hu" # else # define SCNuFAST16 "u" # endif #endif #if !defined SCNxFAST16 || @PRI_MACROS_BROKEN@ # undef SCNxFAST16 # if UINT_FAST16_MAX > UINT32_MAX # define SCNxFAST16 SCNx64 # elif UINT_FAST16_MAX == 0xffff # define SCNxFAST16 "hx" # else # define SCNxFAST16 "x" # endif #endif #if !defined SCNdFAST32 || @PRI_MACROS_BROKEN@ # undef SCNdFAST32 # if INT_FAST32_MAX > INT32_MAX # define SCNdFAST32 SCNd64 # else # define SCNdFAST32 "d" # endif #endif #if !defined SCNiFAST32 || @PRI_MACROS_BROKEN@ # undef SCNiFAST32 # if INT_FAST32_MAX > INT32_MAX # define SCNiFAST32 SCNi64 # else # define SCNiFAST32 "i" # endif #endif #if !defined SCNoFAST32 || @PRI_MACROS_BROKEN@ # undef SCNoFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define SCNoFAST32 SCNo64 # else # define SCNoFAST32 "o" # endif #endif #if !defined SCNuFAST32 || @PRI_MACROS_BROKEN@ # undef SCNuFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define SCNuFAST32 SCNu64 # else # define SCNuFAST32 "u" # endif #endif #if !defined SCNxFAST32 || @PRI_MACROS_BROKEN@ # undef SCNxFAST32 # if UINT_FAST32_MAX > UINT32_MAX # define SCNxFAST32 SCNx64 # else # define SCNxFAST32 "x" # endif #endif #ifdef INT64_MAX # if !defined SCNdFAST64 || @PRI_MACROS_BROKEN@ # undef SCNdFAST64 # define SCNdFAST64 SCNd64 # endif # if !defined SCNiFAST64 || @PRI_MACROS_BROKEN@ # undef SCNiFAST64 # define SCNiFAST64 SCNi64 # endif #endif #ifdef UINT64_MAX # if !defined SCNoFAST64 || @PRI_MACROS_BROKEN@ # undef SCNoFAST64 # define SCNoFAST64 SCNo64 # endif # if !defined SCNuFAST64 || @PRI_MACROS_BROKEN@ # undef SCNuFAST64 # define SCNuFAST64 SCNu64 # endif # if !defined SCNxFAST64 || @PRI_MACROS_BROKEN@ # undef SCNxFAST64 # define SCNxFAST64 SCNx64 # endif #endif #if !defined SCNdMAX || @PRI_MACROS_BROKEN@ # undef SCNdMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define SCNdMAX SCNd64 # else # define SCNdMAX "ld" # endif #endif #if !defined SCNiMAX || @PRI_MACROS_BROKEN@ # undef SCNiMAX # if @INT32_MAX_LT_INTMAX_MAX@ # define SCNiMAX SCNi64 # else # define SCNiMAX "li" # endif #endif #if !defined SCNoMAX || @PRI_MACROS_BROKEN@ # undef SCNoMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define SCNoMAX SCNo64 # else # define SCNoMAX "lo" # endif #endif #if !defined SCNuMAX || @PRI_MACROS_BROKEN@ # undef SCNuMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define SCNuMAX SCNu64 # else # define SCNuMAX "lu" # endif #endif #if !defined SCNxMAX || @PRI_MACROS_BROKEN@ # undef SCNxMAX # if @UINT32_MAX_LT_UINTMAX_MAX@ # define SCNxMAX SCNx64 # else # define SCNxMAX "lx" # endif #endif #if !defined SCNdPTR || @PRI_MACROS_BROKEN@ # undef SCNdPTR # ifdef INTPTR_MAX # define SCNdPTR @PRIPTR_PREFIX@ "d" # endif #endif #if !defined SCNiPTR || @PRI_MACROS_BROKEN@ # undef SCNiPTR # ifdef INTPTR_MAX # define SCNiPTR @PRIPTR_PREFIX@ "i" # endif #endif #if !defined SCNoPTR || @PRI_MACROS_BROKEN@ # undef SCNoPTR # ifdef UINTPTR_MAX # define SCNoPTR @PRIPTR_PREFIX@ "o" # endif #endif #if !defined SCNuPTR || @PRI_MACROS_BROKEN@ # undef SCNuPTR # ifdef UINTPTR_MAX # define SCNuPTR @PRIPTR_PREFIX@ "u" # endif #endif #if !defined SCNxPTR || @PRI_MACROS_BROKEN@ # undef SCNxPTR # ifdef UINTPTR_MAX # define SCNxPTR @PRIPTR_PREFIX@ "x" # endif #endif /* 7.8.2 Functions for greatest-width integer types */ #ifdef __cplusplus extern "C" { #endif #if @GNULIB_IMAXABS@ # if !@HAVE_DECL_IMAXABS@ extern intmax_t imaxabs (intmax_t); # endif #elif defined GNULIB_POSIXCHECK # undef imaxabs # if HAVE_RAW_DECL_IMAXABS _GL_WARN_ON_USE (imaxabs, "imaxabs is unportable - " "use gnulib module imaxabs for portability"); # endif #endif #if @GNULIB_IMAXDIV@ # if !@HAVE_DECL_IMAXDIV@ # if !GNULIB_defined_imaxdiv_t typedef struct { intmax_t quot; intmax_t rem; } imaxdiv_t; # define GNULIB_defined_imaxdiv_t 1 # endif extern imaxdiv_t imaxdiv (intmax_t, intmax_t); # endif #elif defined GNULIB_POSIXCHECK # undef imaxdiv # if HAVE_RAW_DECL_IMAXDIV _GL_WARN_ON_USE (imaxdiv, "imaxdiv is unportable - " "use gnulib module imaxdiv for portability"); # endif #endif #if @GNULIB_STRTOIMAX@ # if @REPLACE_STRTOIMAX@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strtoimax # define strtoimax rpl_strtoimax # endif _GL_FUNCDECL_RPL (strtoimax, intmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strtoimax, intmax_t, (const char *, char **, int)); # else # if !@HAVE_DECL_STRTOIMAX@ # undef strtoimax _GL_FUNCDECL_SYS (strtoimax, intmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoimax, intmax_t, (const char *, char **, int)); # endif _GL_CXXALIASWARN (strtoimax); #elif defined GNULIB_POSIXCHECK # undef strtoimax # if HAVE_RAW_DECL_STRTOIMAX _GL_WARN_ON_USE (strtoimax, "strtoimax is unportable - " "use gnulib module strtoimax for portability"); # endif #endif #if @GNULIB_STRTOUMAX@ # if @REPLACE_STRTOUMAX@ # if !(defined __cplusplus && defined GNULIB_NAMESPACE) # undef strtoumax # define strtoumax rpl_strtoumax # endif _GL_FUNCDECL_RPL (strtoumax, uintmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); _GL_CXXALIAS_RPL (strtoumax, uintmax_t, (const char *, char **, int)); # else # if !@HAVE_DECL_STRTOUMAX@ # undef strtoumax _GL_FUNCDECL_SYS (strtoumax, uintmax_t, (const char *, char **, int) _GL_ARG_NONNULL ((1))); # endif _GL_CXXALIAS_SYS (strtoumax, uintmax_t, (const char *, char **, int)); # endif _GL_CXXALIASWARN (strtoumax); #elif defined GNULIB_POSIXCHECK # undef strtoumax # if HAVE_RAW_DECL_STRTOUMAX _GL_WARN_ON_USE (strtoumax, "strtoumax is unportable - " "use gnulib module strtoumax for portability"); # endif #endif /* Don't bother defining or declaring wcstoimax and wcstoumax, since wide-character functions like this are hardly ever useful. */ #ifdef __cplusplus } #endif #endif /* !defined INTTYPES_H && !defined _GL_JUST_INCLUDE_SYSTEM_INTTYPES_H */ gnuastro-0.5/bootstrapped/lib/intprops.h0000644000175000017500000005061413217200021015436 00000000000000/* intprops.h -- properties of integer types Copyright (C) 2001-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Paul Eggert. */ #ifndef _GL_INTPROPS_H #define _GL_INTPROPS_H #include /* Return a value with the common real type of E and V and the value of V. */ #define _GL_INT_CONVERT(e, v) (0 * (e) + (v)) /* Act like _GL_INT_CONVERT (E, -V) but work around a bug in IRIX 6.5 cc; see . */ #define _GL_INT_NEGATE_CONVERT(e, v) (0 * (e) - (v)) /* The extra casts in the following macros work around compiler bugs, e.g., in Cray C 5.0.3.0. */ /* True if the arithmetic type T is an integer type. bool counts as an integer. */ #define TYPE_IS_INTEGER(t) ((t) 1.5 == 1) /* True if the real type T is signed. */ #define TYPE_SIGNED(t) (! ((t) 0 < (t) -1)) /* Return 1 if the real expression E, after promotion, has a signed or floating type. */ #define EXPR_SIGNED(e) (_GL_INT_NEGATE_CONVERT (e, 1) < 0) /* Minimum and maximum values for integer types and expressions. */ /* The width in bits of the integer type or expression T. Padding bits are not supported; this is checked at compile-time below. */ #define TYPE_WIDTH(t) (sizeof (t) * CHAR_BIT) /* The maximum and minimum values for the integer type T. */ #define TYPE_MINIMUM(t) ((t) ~ TYPE_MAXIMUM (t)) #define TYPE_MAXIMUM(t) \ ((t) (! TYPE_SIGNED (t) \ ? (t) -1 \ : ((((t) 1 << (TYPE_WIDTH (t) - 2)) - 1) * 2 + 1))) /* The maximum and minimum values for the type of the expression E, after integer promotion. E should not have side effects. */ #define _GL_INT_MINIMUM(e) \ (EXPR_SIGNED (e) \ ? ~ _GL_SIGNED_INT_MAXIMUM (e) \ : _GL_INT_CONVERT (e, 0)) #define _GL_INT_MAXIMUM(e) \ (EXPR_SIGNED (e) \ ? _GL_SIGNED_INT_MAXIMUM (e) \ : _GL_INT_NEGATE_CONVERT (e, 1)) #define _GL_SIGNED_INT_MAXIMUM(e) \ (((_GL_INT_CONVERT (e, 1) << (TYPE_WIDTH ((e) + 0) - 2)) - 1) * 2 + 1) /* Work around OpenVMS incompatibility with C99. */ #if !defined LLONG_MAX && defined __INT64_MAX # define LLONG_MAX __INT64_MAX # define LLONG_MIN __INT64_MIN #endif /* This include file assumes that signed types are two's complement without padding bits; the above macros have undefined behavior otherwise. If this is a problem for you, please let us know how to fix it for your host. This assumption is tested by the intprops-tests module. */ /* Does the __typeof__ keyword work? This could be done by 'configure', but for now it's easier to do it by hand. */ #if (2 <= __GNUC__ \ || (1210 <= __IBMC__ && defined __IBM__TYPEOF__) \ || (0x5110 <= __SUNPRO_C && !__STDC__)) # define _GL_HAVE___TYPEOF__ 1 #else # define _GL_HAVE___TYPEOF__ 0 #endif /* Return 1 if the integer type or expression T might be signed. Return 0 if it is definitely unsigned. This macro does not evaluate its argument, and expands to an integer constant expression. */ #if _GL_HAVE___TYPEOF__ # define _GL_SIGNED_TYPE_OR_EXPR(t) TYPE_SIGNED (__typeof__ (t)) #else # define _GL_SIGNED_TYPE_OR_EXPR(t) 1 #endif /* Bound on length of the string representing an unsigned integer value representable in B bits. log10 (2.0) < 146/485. The smallest value of B where this bound is not tight is 2621. */ #define INT_BITS_STRLEN_BOUND(b) (((b) * 146 + 484) / 485) /* Bound on length of the string representing an integer type or expression T. Subtract 1 for the sign bit if T is signed, and then add 1 more for a minus sign if needed. Because _GL_SIGNED_TYPE_OR_EXPR sometimes returns 0 when its argument is signed, this macro may overestimate the true bound by one byte when applied to unsigned types of size 2, 4, 16, ... bytes. */ #define INT_STRLEN_BOUND(t) \ (INT_BITS_STRLEN_BOUND (TYPE_WIDTH (t) - _GL_SIGNED_TYPE_OR_EXPR (t)) \ + _GL_SIGNED_TYPE_OR_EXPR (t)) /* Bound on buffer size needed to represent an integer type or expression T, including the terminating null. */ #define INT_BUFSIZE_BOUND(t) (INT_STRLEN_BOUND (t) + 1) /* Range overflow checks. The INT__RANGE_OVERFLOW macros return 1 if the corresponding C operators might not yield numerically correct answers due to arithmetic overflow. They do not rely on undefined or implementation-defined behavior. Their implementations are simple and straightforward, but they are a bit harder to use than the INT__OVERFLOW macros described below. Example usage: long int i = ...; long int j = ...; if (INT_MULTIPLY_RANGE_OVERFLOW (i, j, LONG_MIN, LONG_MAX)) printf ("multiply would overflow"); else printf ("product is %ld", i * j); Restrictions on *_RANGE_OVERFLOW macros: These macros do not check for all possible numerical problems or undefined or unspecified behavior: they do not check for division by zero, for bad shift counts, or for shifting negative numbers. These macros may evaluate their arguments zero or multiple times, so the arguments should not have side effects. The arithmetic arguments (including the MIN and MAX arguments) must be of the same integer type after the usual arithmetic conversions, and the type must have minimum value MIN and maximum MAX. Unsigned types should use a zero MIN of the proper type. These macros are tuned for constant MIN and MAX. For commutative operations such as A + B, they are also tuned for constant B. */ /* Return 1 if A + B would overflow in [MIN,MAX] arithmetic. See above for restrictions. */ #define INT_ADD_RANGE_OVERFLOW(a, b, min, max) \ ((b) < 0 \ ? (a) < (min) - (b) \ : (max) - (b) < (a)) /* Return 1 if A - B would overflow in [MIN,MAX] arithmetic. See above for restrictions. */ #define INT_SUBTRACT_RANGE_OVERFLOW(a, b, min, max) \ ((b) < 0 \ ? (max) + (b) < (a) \ : (a) < (min) + (b)) /* Return 1 if - A would overflow in [MIN,MAX] arithmetic. See above for restrictions. */ #define INT_NEGATE_RANGE_OVERFLOW(a, min, max) \ ((min) < 0 \ ? (a) < - (max) \ : 0 < (a)) /* Return 1 if A * B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Avoid && and || as they tickle bugs in Sun C 5.11 2010/08/13 and other compilers; see . */ #define INT_MULTIPLY_RANGE_OVERFLOW(a, b, min, max) \ ((b) < 0 \ ? ((a) < 0 \ ? (a) < (max) / (b) \ : (b) == -1 \ ? 0 \ : (min) / (b) < (a)) \ : (b) == 0 \ ? 0 \ : ((a) < 0 \ ? (a) < (min) / (b) \ : (max) / (b) < (a))) /* Return 1 if A / B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Do not check for division by zero. */ #define INT_DIVIDE_RANGE_OVERFLOW(a, b, min, max) \ ((min) < 0 && (b) == -1 && (a) < - (max)) /* Return 1 if A % B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Do not check for division by zero. Mathematically, % should never overflow, but on x86-like hosts INT_MIN % -1 traps, and the C standard permits this, so treat this as an overflow too. */ #define INT_REMAINDER_RANGE_OVERFLOW(a, b, min, max) \ INT_DIVIDE_RANGE_OVERFLOW (a, b, min, max) /* Return 1 if A << B would overflow in [MIN,MAX] arithmetic. See above for restrictions. Here, MIN and MAX are for A only, and B need not be of the same type as the other arguments. The C standard says that behavior is undefined for shifts unless 0 <= B < wordwidth, and that when A is negative then A << B has undefined behavior and A >> B has implementation-defined behavior, but do not check these other restrictions. */ #define INT_LEFT_SHIFT_RANGE_OVERFLOW(a, b, min, max) \ ((a) < 0 \ ? (a) < (min) >> (b) \ : (max) >> (b) < (a)) /* True if __builtin_add_overflow (A, B, P) works when P is non-null. */ #if 5 <= __GNUC__ && !defined __ICC # define _GL_HAS_BUILTIN_OVERFLOW 1 #else # define _GL_HAS_BUILTIN_OVERFLOW 0 #endif /* True if __builtin_add_overflow_p (A, B, C) works. */ #define _GL_HAS_BUILTIN_OVERFLOW_P (7 <= __GNUC__) /* The _GL*_OVERFLOW macros have the same restrictions as the *_RANGE_OVERFLOW macros, except that they do not assume that operands (e.g., A and B) have the same type as MIN and MAX. Instead, they assume that the result (e.g., A + B) has that type. */ #if _GL_HAS_BUILTIN_OVERFLOW_P # define _GL_ADD_OVERFLOW(a, b, min, max) \ __builtin_add_overflow_p (a, b, (__typeof__ ((a) + (b))) 0) # define _GL_SUBTRACT_OVERFLOW(a, b, min, max) \ __builtin_sub_overflow_p (a, b, (__typeof__ ((a) - (b))) 0) # define _GL_MULTIPLY_OVERFLOW(a, b, min, max) \ __builtin_mul_overflow_p (a, b, (__typeof__ ((a) * (b))) 0) #else # define _GL_ADD_OVERFLOW(a, b, min, max) \ ((min) < 0 ? INT_ADD_RANGE_OVERFLOW (a, b, min, max) \ : (a) < 0 ? (b) <= (a) + (b) \ : (b) < 0 ? (a) <= (a) + (b) \ : (a) + (b) < (b)) # define _GL_SUBTRACT_OVERFLOW(a, b, min, max) \ ((min) < 0 ? INT_SUBTRACT_RANGE_OVERFLOW (a, b, min, max) \ : (a) < 0 ? 1 \ : (b) < 0 ? (a) - (b) <= (a) \ : (a) < (b)) # define _GL_MULTIPLY_OVERFLOW(a, b, min, max) \ (((min) == 0 && (((a) < 0 && 0 < (b)) || ((b) < 0 && 0 < (a)))) \ || INT_MULTIPLY_RANGE_OVERFLOW (a, b, min, max)) #endif #define _GL_DIVIDE_OVERFLOW(a, b, min, max) \ ((min) < 0 ? (b) == _GL_INT_NEGATE_CONVERT (min, 1) && (a) < - (max) \ : (a) < 0 ? (b) <= (a) + (b) - 1 \ : (b) < 0 && (a) + (b) <= (a)) #define _GL_REMAINDER_OVERFLOW(a, b, min, max) \ ((min) < 0 ? (b) == _GL_INT_NEGATE_CONVERT (min, 1) && (a) < - (max) \ : (a) < 0 ? (a) % (b) != ((max) - (b) + 1) % (b) \ : (b) < 0 && ! _GL_UNSIGNED_NEG_MULTIPLE (a, b, max)) /* Return a nonzero value if A is a mathematical multiple of B, where A is unsigned, B is negative, and MAX is the maximum value of A's type. A's type must be the same as (A % B)'s type. Normally (A % -B == 0) suffices, but things get tricky if -B would overflow. */ #define _GL_UNSIGNED_NEG_MULTIPLE(a, b, max) \ (((b) < -_GL_SIGNED_INT_MAXIMUM (b) \ ? (_GL_SIGNED_INT_MAXIMUM (b) == (max) \ ? (a) \ : (a) % (_GL_INT_CONVERT (a, _GL_SIGNED_INT_MAXIMUM (b)) + 1)) \ : (a) % - (b)) \ == 0) /* Check for integer overflow, and report low order bits of answer. The INT__OVERFLOW macros return 1 if the corresponding C operators might not yield numerically correct answers due to arithmetic overflow. The INT__WRAPV macros also store the low-order bits of the answer. These macros work correctly on all known practical hosts, and do not rely on undefined behavior due to signed arithmetic overflow. Example usage, assuming A and B are long int: if (INT_MULTIPLY_OVERFLOW (a, b)) printf ("result would overflow\n"); else printf ("result is %ld (no overflow)\n", a * b); Example usage with WRAPV flavor: long int result; bool overflow = INT_MULTIPLY_WRAPV (a, b, &result); printf ("result is %ld (%s)\n", result, overflow ? "after overflow" : "no overflow"); Restrictions on these macros: These macros do not check for all possible numerical problems or undefined or unspecified behavior: they do not check for division by zero, for bad shift counts, or for shifting negative numbers. These macros may evaluate their arguments zero or multiple times, so the arguments should not have side effects. The WRAPV macros are not constant expressions. They support only +, binary -, and *. The result type must be signed. These macros are tuned for their last argument being a constant. Return 1 if the integer expressions A * B, A - B, -A, A * B, A / B, A % B, and A << B would overflow, respectively. */ #define INT_ADD_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_ADD_OVERFLOW) #define INT_SUBTRACT_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_SUBTRACT_OVERFLOW) #if _GL_HAS_BUILTIN_OVERFLOW_P # define INT_NEGATE_OVERFLOW(a) INT_SUBTRACT_OVERFLOW (0, a) #else # define INT_NEGATE_OVERFLOW(a) \ INT_NEGATE_RANGE_OVERFLOW (a, _GL_INT_MINIMUM (a), _GL_INT_MAXIMUM (a)) #endif #define INT_MULTIPLY_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_MULTIPLY_OVERFLOW) #define INT_DIVIDE_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_DIVIDE_OVERFLOW) #define INT_REMAINDER_OVERFLOW(a, b) \ _GL_BINARY_OP_OVERFLOW (a, b, _GL_REMAINDER_OVERFLOW) #define INT_LEFT_SHIFT_OVERFLOW(a, b) \ INT_LEFT_SHIFT_RANGE_OVERFLOW (a, b, \ _GL_INT_MINIMUM (a), _GL_INT_MAXIMUM (a)) /* Return 1 if the expression A B would overflow, where OP_RESULT_OVERFLOW (A, B, MIN, MAX) does the actual test, assuming MIN and MAX are the minimum and maximum for the result type. Arguments should be free of side effects. */ #define _GL_BINARY_OP_OVERFLOW(a, b, op_result_overflow) \ op_result_overflow (a, b, \ _GL_INT_MINIMUM (0 * (b) + (a)), \ _GL_INT_MAXIMUM (0 * (b) + (a))) /* Store the low-order bits of A + B, A - B, A * B, respectively, into *R. Return 1 if the result overflows. See above for restrictions. */ #define INT_ADD_WRAPV(a, b, r) \ _GL_INT_OP_WRAPV (a, b, r, +, __builtin_add_overflow, INT_ADD_OVERFLOW) #define INT_SUBTRACT_WRAPV(a, b, r) \ _GL_INT_OP_WRAPV (a, b, r, -, __builtin_sub_overflow, INT_SUBTRACT_OVERFLOW) #define INT_MULTIPLY_WRAPV(a, b, r) \ _GL_INT_OP_WRAPV (a, b, r, *, __builtin_mul_overflow, INT_MULTIPLY_OVERFLOW) /* Nonzero if this compiler has GCC bug 68193 or Clang bug 25390. See: https://gcc.gnu.org/bugzilla/show_bug.cgi?id=68193 https://llvm.org/bugs/show_bug.cgi?id=25390 For now, assume all versions of GCC-like compilers generate bogus warnings for _Generic. This matters only for older compilers that lack __builtin_add_overflow. */ #if __GNUC__ # define _GL__GENERIC_BOGUS 1 #else # define _GL__GENERIC_BOGUS 0 #endif /* Store the low-order bits of A B into *R, where OP specifies the operation. BUILTIN is the builtin operation, and OVERFLOW the overflow predicate. Return 1 if the result overflows. See above for restrictions. */ #if _GL_HAS_BUILTIN_OVERFLOW # define _GL_INT_OP_WRAPV(a, b, r, op, builtin, overflow) builtin (a, b, r) #elif 201112 <= __STDC_VERSION__ && !_GL__GENERIC_BOGUS # define _GL_INT_OP_WRAPV(a, b, r, op, builtin, overflow) \ (_Generic \ (*(r), \ signed char: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ signed char, SCHAR_MIN, SCHAR_MAX), \ short int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ short int, SHRT_MIN, SHRT_MAX), \ int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ int, INT_MIN, INT_MAX), \ long int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long int, \ long int, LONG_MIN, LONG_MAX), \ long long int: \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long long int, \ long long int, LLONG_MIN, LLONG_MAX))) #else # define _GL_INT_OP_WRAPV(a, b, r, op, builtin, overflow) \ (sizeof *(r) == sizeof (signed char) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ signed char, SCHAR_MIN, SCHAR_MAX) \ : sizeof *(r) == sizeof (short int) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ short int, SHRT_MIN, SHRT_MAX) \ : sizeof *(r) == sizeof (int) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned int, \ int, INT_MIN, INT_MAX) \ : _GL_INT_OP_WRAPV_LONGISH(a, b, r, op, overflow)) # ifdef LLONG_MAX # define _GL_INT_OP_WRAPV_LONGISH(a, b, r, op, overflow) \ (sizeof *(r) == sizeof (long int) \ ? _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long int, \ long int, LONG_MIN, LONG_MAX) \ : _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long long int, \ long long int, LLONG_MIN, LLONG_MAX)) # else # define _GL_INT_OP_WRAPV_LONGISH(a, b, r, op, overflow) \ _GL_INT_OP_CALC (a, b, r, op, overflow, unsigned long int, \ long int, LONG_MIN, LONG_MAX) # endif #endif /* Store the low-order bits of A B into *R, where the operation is given by OP. Use the unsigned type UT for calculation to avoid overflow problems. *R's type is T, with extrema TMIN and TMAX. T must be a signed integer type. Return 1 if the result overflows. */ #define _GL_INT_OP_CALC(a, b, r, op, overflow, ut, t, tmin, tmax) \ (sizeof ((a) op (b)) < sizeof (t) \ ? _GL_INT_OP_CALC1 ((t) (a), (t) (b), r, op, overflow, ut, t, tmin, tmax) \ : _GL_INT_OP_CALC1 (a, b, r, op, overflow, ut, t, tmin, tmax)) #define _GL_INT_OP_CALC1(a, b, r, op, overflow, ut, t, tmin, tmax) \ ((overflow (a, b) \ || (EXPR_SIGNED ((a) op (b)) && ((a) op (b)) < (tmin)) \ || (tmax) < ((a) op (b))) \ ? (*(r) = _GL_INT_OP_WRAPV_VIA_UNSIGNED (a, b, op, ut, t), 1) \ : (*(r) = _GL_INT_OP_WRAPV_VIA_UNSIGNED (a, b, op, ut, t), 0)) /* Return the low-order bits of A B, where the operation is given by OP. Use the unsigned type UT for calculation to avoid undefined behavior on signed integer overflow, and convert the result to type T. UT is at least as wide as T and is no narrower than unsigned int, T is two's complement, and there is no padding or trap representations. Assume that converting UT to T yields the low-order bits, as is done in all known two's-complement C compilers. E.g., see: https://gcc.gnu.org/onlinedocs/gcc/Integers-implementation.html According to the C standard, converting UT to T yields an implementation-defined result or signal for values outside T's range. However, code that works around this theoretical problem runs afoul of a compiler bug in Oracle Studio 12.3 x86. See: https://lists.gnu.org/r/bug-gnulib/2017-04/msg00049.html As the compiler bug is real, don't try to work around the theoretical problem. */ #define _GL_INT_OP_WRAPV_VIA_UNSIGNED(a, b, op, ut, t) \ ((t) ((ut) (a) op (ut) (b))) #endif /* _GL_INTPROPS_H */ gnuastro-0.5/bootstrapped/lib/hard-locale.h0000644000175000017500000000157213217200021015732 00000000000000/* Determine whether a locale is hard. Copyright (C) 1999, 2003-2004, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef HARD_LOCALE_H_ # define HARD_LOCALE_H_ 1 # include bool hard_locale (int); #endif /* HARD_LOCALE_H_ */ gnuastro-0.5/bootstrapped/lib/getopt_int.h0000644000175000017500000001006313217200021015726 00000000000000/* Internal declarations for getopt. Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of the GNU C Library and is also part of gnulib. Patches to this file should be submitted to both projects. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _GETOPT_INT_H #define _GETOPT_INT_H 1 #include extern int _getopt_internal (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, int __long_only, int __posixly_correct); /* Reentrant versions which can handle parsing multiple argument vectors at the same time. */ /* Describe how to deal with options that follow non-option ARGV-elements. REQUIRE_ORDER means don't recognize them as options; stop option processing when the first non-option is seen. This is what POSIX specifies should happen. PERMUTE means permute the contents of ARGV as we scan, so that eventually all the non-options are at the end. This allows options to be given in any order, even with programs that were not written to expect this. RETURN_IN_ORDER is an option available to programs that were written to expect options and other ARGV-elements in any order and that care about the ordering of the two. We describe each non-option ARGV-element as if it were the argument of an option with character code 1. The special argument '--' forces an end of option-scanning regardless of the value of 'ordering'. In the case of RETURN_IN_ORDER, only '--' can cause 'getopt' to return -1 with 'optind' != ARGC. */ enum __ord { REQUIRE_ORDER, PERMUTE, RETURN_IN_ORDER }; /* Data type for reentrant functions. */ struct _getopt_data { /* These have exactly the same meaning as the corresponding global variables, except that they are used for the reentrant versions of getopt. */ int optind; int opterr; int optopt; char *optarg; /* Internal members. */ /* True if the internal members have been initialized. */ int __initialized; /* The next char to be scanned in the option-element in which the last option character we returned was found. This allows us to pick up the scan where we left off. If this is zero, or a null string, it means resume the scan by advancing to the next ARGV-element. */ char *__nextchar; /* See __ord above. */ enum __ord __ordering; /* Handle permutation of arguments. */ /* Describe the part of ARGV that contains non-options that have been skipped. 'first_nonopt' is the index in ARGV of the first of them; 'last_nonopt' is the index after the last of them. */ int __first_nonopt; int __last_nonopt; }; /* The initializer is necessary to set OPTIND and OPTERR to their default values and to clear the initialization flag. */ #define _GETOPT_DATA_INITIALIZER { 1, 1 } extern int _getopt_internal_r (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, int __long_only, struct _getopt_data *__data, int __posixly_correct); extern int _getopt_long_r (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, struct _getopt_data *__data); extern int _getopt_long_only_r (int ___argc, char **___argv, const char *__shortopts, const struct option *__longopts, int *__longind, struct _getopt_data *__data); #endif /* getopt_int.h */ gnuastro-0.5/bootstrapped/lib/getopt.in.h0000644000175000017500000000406313217200021015464 00000000000000/* Declarations for getopt. Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of gnulib. Unlike most of the getopt implementation, it is NOT shared with the GNU C Library, which supplies a different version of this file. This file is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This file is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with gnulib; if not, see . */ #ifndef _@GUARD_PREFIX@_GETOPT_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. We must also inform the replacement unistd.h to not recursively use ; our definitions will be present soon enough. */ #if @HAVE_GETOPT_H@ # define _GL_SYSTEM_GETOPT # @INCLUDE_NEXT@ @NEXT_GETOPT_H@ # undef _GL_SYSTEM_GETOPT #endif #define _@GUARD_PREFIX@_GETOPT_H 1 /* Standalone applications should #define __GETOPT_PREFIX to an identifier that prefixes the external functions and variables defined in getopt-core.h and getopt-ext.h. When this happens, include the headers that might declare getopt so that they will not cause confusion if included after this file (if the system had , we have already included it). */ #if defined __GETOPT_PREFIX # if !@HAVE_GETOPT_H@ # define __need_system_stdlib_h # include # undef __need_system_stdlib_h # include # include # endif #endif /* The definition of _GL_ARG_NONNULL is copied here. */ #include #include #include #endif /* _@GUARD_PREFIX@_GETOPT_H */ gnuastro-0.5/bootstrapped/lib/getopt-pfx-ext.h0000644000175000017500000000533213217200021016450 00000000000000/* getopt (GNU extensions) gnulib wrapper header. Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of gnulib. Unlike most of the getopt implementation, it is NOT shared with the GNU C Library. This file is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This file is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with gnulib; if not, see . */ #ifndef _GETOPT_PFX_EXT_H #define _GETOPT_PFX_EXT_H 1 /* This header should not be used directly; include getopt.h instead. It does not have a protective #error, because the guard macro for getopt.h in gnulib is not fixed. */ /* Standalone applications should #define __GETOPT_PREFIX to an identifier that prefixes the external functions and variables defined in getopt-core.h and getopt-ext.h. Systematically rename identifiers so that they do not collide with the system functions and variables. Renaming avoids problems with some compilers and linkers. */ #ifdef __GETOPT_PREFIX # ifndef __GETOPT_ID # define __GETOPT_CONCAT(x, y) x ## y # define __GETOPT_XCONCAT(x, y) __GETOPT_CONCAT (x, y) # define __GETOPT_ID(y) __GETOPT_XCONCAT (__GETOPT_PREFIX, y) # endif # undef getopt_long # undef getopt_long_only # undef option # undef _getopt_internal # define getopt_long __GETOPT_ID (getopt_long) # define getopt_long_only __GETOPT_ID (getopt_long_only) # define option __GETOPT_ID (option) # define _getopt_internal __GETOPT_ID (getopt_internal) /* The system's getopt.h may have already included getopt-ext.h to declare the unprefixed identifiers. Undef _GETOPT_EXT_H so that getopt-ext.h declares them with prefixes. */ # undef _GETOPT_EXT_H #endif /* Standalone applications get correct prototypes for getopt_long and getopt_long_only; they declare "char **argv". For backward compatibility with old applications, if __GETOPT_PREFIX is not defined, we supply GNU-libc-compatible, but incorrect, prototypes using "char *const *argv". (GNU libc is stuck with the incorrect prototypes, as they are baked into older versions of LSB.) */ #ifndef __getopt_argv_const # if defined __GETOPT_PREFIX # define __getopt_argv_const /* empty */ # else # define __getopt_argv_const const # endif #endif #include #endif /* _GETOPT_PFX_EXT_H */ gnuastro-0.5/bootstrapped/lib/getopt-pfx-core.h0000644000175000017500000000426213217200021016601 00000000000000/* getopt (basic, portable features) gnulib wrapper header. Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of gnulib. Unlike most of the getopt implementation, it is NOT shared with the GNU C Library. This file is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This file is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with gnulib; if not, see . */ #ifndef _GETOPT_PFX_CORE_H #define _GETOPT_PFX_CORE_H 1 /* This header should not be used directly; include getopt.h or unistd.h instead. It does not have a protective #error, because the guard macro for getopt.h in gnulib is not fixed. */ /* Standalone applications should #define __GETOPT_PREFIX to an identifier that prefixes the external functions and variables defined in getopt-core.h and getopt-ext.h. Systematically rename identifiers so that they do not collide with the system functions and variables. Renaming avoids problems with some compilers and linkers. */ #ifdef __GETOPT_PREFIX # ifndef __GETOPT_ID # define __GETOPT_CONCAT(x, y) x ## y # define __GETOPT_XCONCAT(x, y) __GETOPT_CONCAT (x, y) # define __GETOPT_ID(y) __GETOPT_XCONCAT (__GETOPT_PREFIX, y) # endif # undef getopt # undef optarg # undef opterr # undef optind # undef optopt # define getopt __GETOPT_ID (getopt) # define optarg __GETOPT_ID (optarg) # define opterr __GETOPT_ID (opterr) # define optind __GETOPT_ID (optind) # define optopt __GETOPT_ID (optopt) /* The system's getopt.h may have already included getopt-core.h to declare the unprefixed identifiers. Undef _GETOPT_CORE_H so that getopt-core.h declares them with prefixes. */ # undef _GETOPT_CORE_H #endif #include #endif /* _GETOPT_PFX_CORE_H */ gnuastro-0.5/bootstrapped/lib/getopt-ext.h0000644000175000017500000000572413217200021015662 00000000000000/* Declarations for getopt (GNU extensions). Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of the GNU C Library and is also part of gnulib. Patches to this file should be submitted to both projects. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _GETOPT_EXT_H #define _GETOPT_EXT_H 1 /* This header should not be used directly; include getopt.h instead. Unlike most bits headers, it does not have a protective #error, because the guard macro for getopt.h in gnulib is not fixed. */ __BEGIN_DECLS /* Describe the long-named options requested by the application. The LONG_OPTIONS argument to getopt_long or getopt_long_only is a vector of 'struct option' terminated by an element containing a name which is zero. The field 'has_arg' is: no_argument (or 0) if the option does not take an argument, required_argument (or 1) if the option requires an argument, optional_argument (or 2) if the option takes an optional argument. If the field 'flag' is not NULL, it points to a variable that is set to the value given in the field 'val' when the option is found, but left unchanged if the option is not found. To have a long-named option do something other than set an 'int' to a compiled-in constant, such as set a value from 'optarg', set the option's 'flag' field to zero and its 'val' field to a nonzero value (the equivalent single-letter option character, if there is one). For long options that have a zero 'flag' field, 'getopt' returns the contents of the 'val' field. */ struct option { const char *name; /* has_arg can't be an enum because some compilers complain about type mismatches in all the code that assumes it is an int. */ int has_arg; int *flag; int val; }; /* Names for the values of the 'has_arg' field of 'struct option'. */ #define no_argument 0 #define required_argument 1 #define optional_argument 2 extern int getopt_long (int ___argc, char *__getopt_argv_const *___argv, const char *__shortopts, const struct option *__longopts, int *__longind) __THROW _GL_ARG_NONNULL ((2, 3)); extern int getopt_long_only (int ___argc, char *__getopt_argv_const *___argv, const char *__shortopts, const struct option *__longopts, int *__longind) __THROW _GL_ARG_NONNULL ((2, 3)); __END_DECLS #endif /* _GETOPT_EXT_H */ gnuastro-0.5/bootstrapped/lib/getopt-core.h0000644000175000017500000000710313217200021016003 00000000000000/* Declarations for getopt (basic, portable features only). Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of the GNU C Library and is also part of gnulib. Patches to this file should be submitted to both projects. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _GETOPT_CORE_H #define _GETOPT_CORE_H 1 /* This header should not be used directly; include getopt.h or unistd.h instead. Unlike most bits headers, it does not have a protective #error, because the guard macro for getopt.h in gnulib is not fixed. */ __BEGIN_DECLS /* For communication from 'getopt' to the caller. When 'getopt' finds an option that takes an argument, the argument value is returned here. Also, when 'ordering' is RETURN_IN_ORDER, each non-option ARGV-element is returned here. */ extern char *optarg; /* Index in ARGV of the next element to be scanned. This is used for communication to and from the caller and for communication between successive calls to 'getopt'. On entry to 'getopt', zero means this is the first call; initialize. When 'getopt' returns -1, this is the index of the first of the non-option elements that the caller should itself scan. Otherwise, 'optind' communicates from one call to the next how much of ARGV has been scanned so far. */ extern int optind; /* Callers store zero here to inhibit the error message 'getopt' prints for unrecognized options. */ extern int opterr; /* Set to an option character which was unrecognized. */ extern int optopt; /* Get definitions and prototypes for functions to process the arguments in ARGV (ARGC of them, minus the program name) for options given in OPTS. Return the option character from OPTS just read. Return -1 when there are no more options. For unrecognized options, or options missing arguments, 'optopt' is set to the option letter, and '?' is returned. The OPTS string is a list of characters which are recognized option letters, optionally followed by colons, specifying that that letter takes an argument, to be placed in 'optarg'. If a letter in OPTS is followed by two colons, its argument is optional. This behavior is specific to the GNU 'getopt'. The argument '--' causes premature termination of argument scanning, explicitly telling 'getopt' that there are no more options. If OPTS begins with '-', then non-option arguments are treated as arguments to the option '\1'. This behavior is specific to the GNU 'getopt'. If OPTS begins with '+', or POSIXLY_CORRECT is set in the environment, then do not permute arguments. For standards compliance, the 'argv' argument has the type char *const *, but this is inaccurate; if argument permutation is enabled, the argv array (not the strings it points to) must be writable. */ extern int getopt (int ___argc, char *const *___argv, const char *__shortopts) __THROW _GL_ARG_NONNULL ((2, 3)); __END_DECLS #endif /* _GETOPT_CORE_H */ gnuastro-0.5/bootstrapped/lib/getopt-cdefs.in.h0000644000175000017500000000376113217200021016552 00000000000000/* getopt-on-non-glibc compatibility macros. Copyright (C) 1989-2017 Free Software Foundation, Inc. This file is part of gnulib. Unlike most of the getopt implementation, it is NOT shared with the GNU C Library. This file is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This file is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with gnulib; if not, see . */ #ifndef _GETOPT_CDEFS_H #define _GETOPT_CDEFS_H 1 /* This header should not be used directly; include getopt.h or unistd.h instead. It does not have a protective #error, because the guard macro for getopt.h in gnulib is not fixed. */ /* getopt-core.h and getopt-ext.h are shared with GNU libc, and expect a number of the internal macros supplied to GNU libc's headers by sys/cdefs.h. Provide fallback definitions for all of them. */ #if @HAVE_SYS_CDEFS_H@ # include #endif #ifndef __BEGIN_DECLS # ifdef __cplusplus # define __BEGIN_DECLS extern "C" { # else # define __BEGIN_DECLS /* nothing */ # endif #endif #ifndef __END_DECLS # ifdef __cplusplus # define __END_DECLS } # else # define __END_DECLS /* nothing */ # endif #endif #ifndef __GNUC_PREREQ # if defined __GNUC__ && defined __GNUC_VERSION__ # define __GNUC_PREREQ(maj, min) \ ((__GNUC__ << 16) + __GNUC_MINOR__ >= ((maj) << 16) + (min)) # else # define __GNUC_PREREQ(maj, min) 0 # endif #endif #ifndef __THROW # if defined __cplusplus && __GNUC_PREREQ (2,8) # define __THROW throw () # else # define __THROW # endif #endif #endif /* _GETOPT_CDEFS_H */ gnuastro-0.5/bootstrapped/lib/float.in.h0000644000175000017500000001677713217200021015306 00000000000000/* A correct . Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _@GUARD_PREFIX@_FLOAT_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_FLOAT_H@ #ifndef _@GUARD_PREFIX@_FLOAT_H #define _@GUARD_PREFIX@_FLOAT_H /* 'long double' properties. */ #if defined __i386__ && (defined __BEOS__ || defined __OpenBSD__) /* Number of mantissa units, in base FLT_RADIX. */ # undef LDBL_MANT_DIG # define LDBL_MANT_DIG 64 /* Number of decimal digits that is sufficient for representing a number. */ # undef LDBL_DIG # define LDBL_DIG 18 /* x-1 where x is the smallest representable number > 1. */ # undef LDBL_EPSILON # define LDBL_EPSILON 1.0842021724855044340E-19L /* Minimum e such that FLT_RADIX^(e-1) is a normalized number. */ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP (-16381) /* Maximum e such that FLT_RADIX^(e-1) is a representable finite number. */ # undef LDBL_MAX_EXP # define LDBL_MAX_EXP 16384 /* Minimum positive normalized number. */ # undef LDBL_MIN # define LDBL_MIN 3.3621031431120935063E-4932L /* Maximum representable finite number. */ # undef LDBL_MAX # define LDBL_MAX 1.1897314953572317650E+4932L /* Minimum e such that 10^e is in the range of normalized numbers. */ # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP (-4931) /* Maximum e such that 10^e is in the range of representable finite numbers. */ # undef LDBL_MAX_10_EXP # define LDBL_MAX_10_EXP 4932 #endif /* On FreeBSD/x86 6.4, the 'long double' type really has only 53 bits of precision in the compiler but 64 bits of precision at runtime. See . */ #if defined __i386__ && (defined __FreeBSD__ || defined __DragonFly__) /* Number of mantissa units, in base FLT_RADIX. */ # undef LDBL_MANT_DIG # define LDBL_MANT_DIG 64 /* Number of decimal digits that is sufficient for representing a number. */ # undef LDBL_DIG # define LDBL_DIG 18 /* x-1 where x is the smallest representable number > 1. */ # undef LDBL_EPSILON # define LDBL_EPSILON 1.084202172485504434007452800869941711426e-19L /* 2^-63 */ /* Minimum e such that FLT_RADIX^(e-1) is a normalized number. */ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP (-16381) /* Maximum e such that FLT_RADIX^(e-1) is a representable finite number. */ # undef LDBL_MAX_EXP # define LDBL_MAX_EXP 16384 /* Minimum positive normalized number. */ # undef LDBL_MIN # define LDBL_MIN 3.362103143112093506262677817321752E-4932L /* = 0x1p-16382L */ /* Maximum representable finite number. */ # undef LDBL_MAX /* LDBL_MAX is represented as { 0xFFFFFFFF, 0xFFFFFFFF, 32766 }. But the largest literal that GCC allows us to write is 0x0.fffffffffffff8p16384L = { 0xFFFFF800, 0xFFFFFFFF, 32766 }. So, define it like this through a reference to an external variable const unsigned int LDBL_MAX[3] = { 0xFFFFFFFF, 0xFFFFFFFF, 32766 }; extern const long double LDBL_MAX; Unfortunately, this is not a constant expression. */ union gl_long_double_union { struct { unsigned int lo; unsigned int hi; unsigned int exponent; } xd; long double ld; }; extern const union gl_long_double_union gl_LDBL_MAX; # define LDBL_MAX (gl_LDBL_MAX.ld) /* Minimum e such that 10^e is in the range of normalized numbers. */ # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP (-4931) /* Maximum e such that 10^e is in the range of representable finite numbers. */ # undef LDBL_MAX_10_EXP # define LDBL_MAX_10_EXP 4932 #endif /* On AIX 7.1 with gcc 4.2, the values of LDBL_MIN_EXP, LDBL_MIN, LDBL_MAX are wrong. On Linux/PowerPC with gcc 4.4, the value of LDBL_MAX is wrong. */ #if (defined _ARCH_PPC || defined _POWER) && defined _AIX && (LDBL_MANT_DIG == 106) && defined __GNUC__ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP DBL_MIN_EXP # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP DBL_MIN_10_EXP # undef LDBL_MIN # define LDBL_MIN 2.22507385850720138309023271733240406422e-308L /* DBL_MIN = 2^-1022 */ #endif #if (defined _ARCH_PPC || defined _POWER) && (defined _AIX || defined __linux__) && (LDBL_MANT_DIG == 106) && defined __GNUC__ # undef LDBL_MAX /* LDBL_MAX is represented as { 0x7FEFFFFF, 0xFFFFFFFF, 0x7C8FFFFF, 0xFFFFFFFF }. It is not easy to define: #define LDBL_MAX 1.79769313486231580793728971405302307166e308L is too small, whereas #define LDBL_MAX 1.79769313486231580793728971405302307167e308L is too large. Apparently a bug in GCC decimal-to-binary conversion. Also, I can't get values larger than #define LDBL63 ((long double) (1ULL << 63)) #define LDBL882 (LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63) #define LDBL945 (LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63) #define LDBL1008 (LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63 * LDBL63) #define LDBL_MAX (LDBL1008 * 65535.0L + LDBL945 * (long double) 9223372036821221375ULL + LDBL882 * (long double) 4611686018427387904ULL) which is represented as { 0x7FEFFFFF, 0xFFFFFFFF, 0x7C8FFFFF, 0xF8000000 }. So, define it like this through a reference to an external variable const double LDBL_MAX[2] = { DBL_MAX, DBL_MAX / (double)134217728UL / (double)134217728UL }; extern const long double LDBL_MAX; or through a pointer cast #define LDBL_MAX \ (*(const long double *) (double[]) { DBL_MAX, DBL_MAX / (double)134217728UL / (double)134217728UL }) Unfortunately, this is not a constant expression, and the latter expression does not work well when GCC is optimizing.. */ union gl_long_double_union { struct { double hi; double lo; } dd; long double ld; }; extern const union gl_long_double_union gl_LDBL_MAX; # define LDBL_MAX (gl_LDBL_MAX.ld) #endif /* On IRIX 6.5, with cc, the value of LDBL_MANT_DIG is wrong. On IRIX 6.5, with gcc 4.2, the values of LDBL_MIN_EXP, LDBL_MIN, LDBL_EPSILON are wrong. */ #if defined __sgi && (LDBL_MANT_DIG >= 106) # undef LDBL_MANT_DIG # define LDBL_MANT_DIG 106 # if defined __GNUC__ # undef LDBL_MIN_EXP # define LDBL_MIN_EXP DBL_MIN_EXP # undef LDBL_MIN_10_EXP # define LDBL_MIN_10_EXP DBL_MIN_10_EXP # undef LDBL_MIN # define LDBL_MIN 2.22507385850720138309023271733240406422e-308L /* DBL_MIN = 2^-1022 */ # undef LDBL_EPSILON # define LDBL_EPSILON 2.46519032881566189191165176650870696773e-32L /* 2^-105 */ # endif #endif #if @REPLACE_ITOLD@ /* Pull in a function that fixes the 'int' to 'long double' conversion of glibc 2.7. */ extern # ifdef __cplusplus "C" # endif void _Qp_itoq (long double *, int); static void (*_gl_float_fix_itold) (long double *, int) = _Qp_itoq; #endif #endif /* _@GUARD_PREFIX@_FLOAT_H */ #endif /* _@GUARD_PREFIX@_FLOAT_H */ gnuastro-0.5/bootstrapped/lib/error.h0000644000175000017500000000553313217200021014711 00000000000000/* Declaration for error-reporting function Copyright (C) 1995-1997, 2003, 2006, 2008-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _ERROR_H #define _ERROR_H 1 /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif /* On mingw, the flavor of printf depends on whether the extensions module * is in use; the check for determines the witness macro. */ #ifndef _GL_ATTRIBUTE_SPEC_PRINTF # if GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU # define _GL_ATTRIBUTE_SPEC_PRINTF __gnu_printf__ # else # define _GL_ATTRIBUTE_SPEC_PRINTF __printf__ # endif #endif #ifdef __cplusplus extern "C" { #endif /* Print a message with 'fprintf (stderr, FORMAT, ...)'; if ERRNUM is nonzero, follow it with ": " and strerror (ERRNUM). If STATUS is nonzero, terminate the program with 'exit (STATUS)'. */ extern void error (int __status, int __errnum, const char *__format, ...) _GL_ATTRIBUTE_FORMAT ((_GL_ATTRIBUTE_SPEC_PRINTF, 3, 4)); extern void error_at_line (int __status, int __errnum, const char *__fname, unsigned int __lineno, const char *__format, ...) _GL_ATTRIBUTE_FORMAT ((_GL_ATTRIBUTE_SPEC_PRINTF, 5, 6)); /* If NULL, error will flush stdout, then print on stderr the program name, a colon and a space. Otherwise, error will call this function without parameters instead. */ extern void (*error_print_progname) (void); /* This variable is incremented each time 'error' is called. */ extern unsigned int error_message_count; /* Sometimes we want to have at most one error per line. This variable controls whether this mode is selected or not. */ extern int error_one_per_line; #ifdef __cplusplus } #endif #endif /* error.h */ gnuastro-0.5/bootstrapped/lib/errno.in.h0000644000175000017500000001646413217200021015317 00000000000000/* A POSIX-like . Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _@GUARD_PREFIX@_ERRNO_H #if __GNUC__ >= 3 @PRAGMA_SYSTEM_HEADER@ #endif @PRAGMA_COLUMNS@ /* The include_next requires a split double-inclusion guard. */ #@INCLUDE_NEXT@ @NEXT_ERRNO_H@ #ifndef _@GUARD_PREFIX@_ERRNO_H #define _@GUARD_PREFIX@_ERRNO_H /* On native Windows platforms, many macros are not defined. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* These are the same values as defined by MSVC 10, for interoperability. */ # ifndef ENOMSG # define ENOMSG 122 # define GNULIB_defined_ENOMSG 1 # endif # ifndef EIDRM # define EIDRM 111 # define GNULIB_defined_EIDRM 1 # endif # ifndef ENOLINK # define ENOLINK 121 # define GNULIB_defined_ENOLINK 1 # endif # ifndef EPROTO # define EPROTO 134 # define GNULIB_defined_EPROTO 1 # endif # ifndef EBADMSG # define EBADMSG 104 # define GNULIB_defined_EBADMSG 1 # endif # ifndef EOVERFLOW # define EOVERFLOW 132 # define GNULIB_defined_EOVERFLOW 1 # endif # ifndef ENOTSUP # define ENOTSUP 129 # define GNULIB_defined_ENOTSUP 1 # endif # ifndef ENETRESET # define ENETRESET 117 # define GNULIB_defined_ENETRESET 1 # endif # ifndef ECONNABORTED # define ECONNABORTED 106 # define GNULIB_defined_ECONNABORTED 1 # endif # ifndef ECANCELED # define ECANCELED 105 # define GNULIB_defined_ECANCELED 1 # endif # ifndef EOWNERDEAD # define EOWNERDEAD 133 # define GNULIB_defined_EOWNERDEAD 1 # endif # ifndef ENOTRECOVERABLE # define ENOTRECOVERABLE 127 # define GNULIB_defined_ENOTRECOVERABLE 1 # endif # ifndef EINPROGRESS # define EINPROGRESS 112 # define EALREADY 103 # define ENOTSOCK 128 # define EDESTADDRREQ 109 # define EMSGSIZE 115 # define EPROTOTYPE 136 # define ENOPROTOOPT 123 # define EPROTONOSUPPORT 135 # define EOPNOTSUPP 130 # define EAFNOSUPPORT 102 # define EADDRINUSE 100 # define EADDRNOTAVAIL 101 # define ENETDOWN 116 # define ENETUNREACH 118 # define ECONNRESET 108 # define ENOBUFS 119 # define EISCONN 113 # define ENOTCONN 126 # define ETIMEDOUT 138 # define ECONNREFUSED 107 # define ELOOP 114 # define EHOSTUNREACH 110 # define EWOULDBLOCK 140 # define GNULIB_defined_ESOCK 1 # endif # ifndef ETXTBSY # define ETXTBSY 139 # define ENODATA 120 /* not required by POSIX */ # define ENOSR 124 /* not required by POSIX */ # define ENOSTR 125 /* not required by POSIX */ # define ETIME 137 /* not required by POSIX */ # define EOTHER 131 /* not required by POSIX */ # define GNULIB_defined_ESTREAMS 1 # endif /* These are intentionally the same values as the WSA* error numbers, defined in . */ # define ESOCKTNOSUPPORT 10044 /* not required by POSIX */ # define EPFNOSUPPORT 10046 /* not required by POSIX */ # define ESHUTDOWN 10058 /* not required by POSIX */ # define ETOOMANYREFS 10059 /* not required by POSIX */ # define EHOSTDOWN 10064 /* not required by POSIX */ # define EPROCLIM 10067 /* not required by POSIX */ # define EUSERS 10068 /* not required by POSIX */ # define EDQUOT 10069 # define ESTALE 10070 # define EREMOTE 10071 /* not required by POSIX */ # define GNULIB_defined_EWINSOCK 1 # endif /* On OSF/1 5.1, when _XOPEN_SOURCE_EXTENDED is not defined, the macros EMULTIHOP, ENOLINK, EOVERFLOW are not defined. */ # if @EMULTIHOP_HIDDEN@ # define EMULTIHOP @EMULTIHOP_VALUE@ # define GNULIB_defined_EMULTIHOP 1 # endif # if @ENOLINK_HIDDEN@ # define ENOLINK @ENOLINK_VALUE@ # define GNULIB_defined_ENOLINK 1 # endif # if @EOVERFLOW_HIDDEN@ # define EOVERFLOW @EOVERFLOW_VALUE@ # define GNULIB_defined_EOVERFLOW 1 # endif /* On OpenBSD 4.0 and on native Windows, the macros ENOMSG, EIDRM, ENOLINK, EPROTO, EMULTIHOP, EBADMSG, EOVERFLOW, ENOTSUP, ECANCELED are not defined. Likewise, on NonStop Kernel, EDQUOT is not defined. Define them here. Values >= 2000 seem safe to use: Solaris ESTALE = 151, HP-UX EWOULDBLOCK = 246, IRIX EDQUOT = 1133. Note: When one of these systems defines some of these macros some day, binaries will have to be recompiled so that they recognizes the new errno values from the system. */ # ifndef ENOMSG # define ENOMSG 2000 # define GNULIB_defined_ENOMSG 1 # endif # ifndef EIDRM # define EIDRM 2001 # define GNULIB_defined_EIDRM 1 # endif # ifndef ENOLINK # define ENOLINK 2002 # define GNULIB_defined_ENOLINK 1 # endif # ifndef EPROTO # define EPROTO 2003 # define GNULIB_defined_EPROTO 1 # endif # ifndef EMULTIHOP # define EMULTIHOP 2004 # define GNULIB_defined_EMULTIHOP 1 # endif # ifndef EBADMSG # define EBADMSG 2005 # define GNULIB_defined_EBADMSG 1 # endif # ifndef EOVERFLOW # define EOVERFLOW 2006 # define GNULIB_defined_EOVERFLOW 1 # endif # ifndef ENOTSUP # define ENOTSUP 2007 # define GNULIB_defined_ENOTSUP 1 # endif # ifndef ENETRESET # define ENETRESET 2011 # define GNULIB_defined_ENETRESET 1 # endif # ifndef ECONNABORTED # define ECONNABORTED 2012 # define GNULIB_defined_ECONNABORTED 1 # endif # ifndef ESTALE # define ESTALE 2009 # define GNULIB_defined_ESTALE 1 # endif # ifndef EDQUOT # define EDQUOT 2010 # define GNULIB_defined_EDQUOT 1 # endif # ifndef ECANCELED # define ECANCELED 2008 # define GNULIB_defined_ECANCELED 1 # endif /* On many platforms, the macros EOWNERDEAD and ENOTRECOVERABLE are not defined. */ # ifndef EOWNERDEAD # if defined __sun /* Use the same values as defined for Solaris >= 8, for interoperability. */ # define EOWNERDEAD 58 # define ENOTRECOVERABLE 59 # elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* We have a conflict here: pthreads-win32 defines these values differently than MSVC 10. It's hairy to decide which one to use. */ # if defined __MINGW32__ && !defined USE_WINDOWS_THREADS /* Use the same values as defined by pthreads-win32, for interoperability. */ # define EOWNERDEAD 43 # define ENOTRECOVERABLE 44 # else /* Use the same values as defined by MSVC 10, for interoperability. */ # define EOWNERDEAD 133 # define ENOTRECOVERABLE 127 # endif # else # define EOWNERDEAD 2013 # define ENOTRECOVERABLE 2014 # endif # define GNULIB_defined_EOWNERDEAD 1 # define GNULIB_defined_ENOTRECOVERABLE 1 # endif # ifndef EILSEQ # define EILSEQ 2015 # define GNULIB_defined_EILSEQ 1 # endif #endif /* _@GUARD_PREFIX@_ERRNO_H */ #endif /* _@GUARD_PREFIX@_ERRNO_H */ gnuastro-0.5/bootstrapped/lib/dosname.h0000644000175000017500000000373413217200021015207 00000000000000/* File names on MS-DOS/Windows systems. Copyright (C) 2000-2001, 2004-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . From Paul Eggert and Jim Meyering. */ #ifndef _DOSNAME_H #define _DOSNAME_H #if (defined _WIN32 || defined __WIN32__ || \ defined __MSDOS__ || defined __CYGWIN__ || \ defined __EMX__ || defined __DJGPP__) /* This internal macro assumes ASCII, but all hosts that support drive letters use ASCII. */ # define _IS_DRIVE_LETTER(C) (((unsigned int) (C) | ('a' - 'A')) - 'a' \ <= 'z' - 'a') # define FILE_SYSTEM_PREFIX_LEN(Filename) \ (_IS_DRIVE_LETTER ((Filename)[0]) && (Filename)[1] == ':' ? 2 : 0) # ifndef __CYGWIN__ # define FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE 1 # endif # define ISSLASH(C) ((C) == '/' || (C) == '\\') #else # define FILE_SYSTEM_PREFIX_LEN(Filename) 0 # define ISSLASH(C) ((C) == '/') #endif #ifndef FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE # define FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE 0 #endif #if FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE # define IS_ABSOLUTE_FILE_NAME(F) ISSLASH ((F)[FILE_SYSTEM_PREFIX_LEN (F)]) # else # define IS_ABSOLUTE_FILE_NAME(F) \ (ISSLASH ((F)[0]) || FILE_SYSTEM_PREFIX_LEN (F) != 0) #endif #define IS_RELATIVE_FILE_NAME(F) (! IS_ABSOLUTE_FILE_NAME (F)) #endif /* DOSNAME_H_ */ gnuastro-0.5/bootstrapped/lib/dirname.h0000644000175000017500000000300013217200021015162 00000000000000/* Take file names apart into directory and base names. Copyright (C) 1998, 2001, 2003-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef DIRNAME_H_ # define DIRNAME_H_ 1 # include # include # include "dosname.h" # ifndef DIRECTORY_SEPARATOR # define DIRECTORY_SEPARATOR '/' # endif # ifndef DOUBLE_SLASH_IS_DISTINCT_ROOT # define DOUBLE_SLASH_IS_DISTINCT_ROOT 0 # endif #ifdef __cplusplus extern "C" { #endif # if GNULIB_DIRNAME char *base_name (char const *file); char *dir_name (char const *file); # endif char *mdir_name (char const *file); size_t base_len (char const *file) _GL_ATTRIBUTE_PURE; size_t dir_len (char const *file) _GL_ATTRIBUTE_PURE; char *last_component (char const *file) _GL_ATTRIBUTE_PURE; bool strip_trailing_slashes (char *file); #ifdef __cplusplus } /* extern "C" */ #endif #endif /* not DIRNAME_H_ */ gnuastro-0.5/bootstrapped/lib/alloca.in.h0000644000175000017500000000400213217200020015405 00000000000000/* Memory allocation on the stack. Copyright (C) 1995, 1999, 2001-2004, 2006-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Avoid using the symbol _ALLOCA_H here, as Bison assumes _ALLOCA_H means there is a real alloca function. */ #ifndef _GL_ALLOCA_H #define _GL_ALLOCA_H /* alloca (N) returns a pointer to N bytes of memory allocated on the stack, which will last until the function returns. Use of alloca should be avoided: - inside arguments of function calls - undefined behaviour, - in inline functions - the allocation may actually last until the calling function returns, - for huge N (say, N >= 65536) - you never know how large (or small) the stack is, and when the stack cannot fulfill the memory allocation request, the program just crashes. */ #ifndef alloca # ifdef __GNUC__ # define alloca __builtin_alloca # elif defined _AIX # define alloca __alloca # elif defined _MSC_VER # include # define alloca _alloca # elif defined __DECC && defined __VMS # define alloca __ALLOCA # elif defined __TANDEM && defined _TNS_E_TARGET # ifdef __cplusplus extern "C" # endif void *_alloca (unsigned short); # pragma intrinsic (_alloca) # define alloca _alloca # elif defined __MVS__ # include # else # include # ifdef __cplusplus extern "C" # endif void *alloca (size_t); # endif #endif #endif /* _GL_ALLOCA_H */ gnuastro-0.5/bootstrapped/lib/wcwidth.c0000644000175000017500000000300013217200022015210 00000000000000/* Determine the number of screen columns needed for a character. Copyright (C) 2006-2007, 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include /* Get iswprint. */ #include #include "localcharset.h" #include "streq.h" #include "uniwidth.h" int wcwidth (wchar_t wc) #undef wcwidth { /* In UTF-8 locales, use a Unicode aware width function. */ const char *encoding = locale_charset (); if (STREQ_OPT (encoding, "UTF-8", 'U', 'T', 'F', '-', '8', 0, 0, 0 ,0)) { /* We assume that in a UTF-8 locale, a wide character is the same as a Unicode character. */ return uc_width (wc, encoding); } else { /* Otherwise, fall back to the system's wcwidth function. */ #if HAVE_WCWIDTH return wcwidth (wc); #else return wc == 0 ? 0 : iswprint (wc) ? 1 : -1; #endif } } gnuastro-0.5/bootstrapped/lib/wcrtomb.c0000644000175000017500000000271613217200022015231 00000000000000/* Convert wide character to multibyte character. Copyright (C) 2008-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include size_t wcrtomb (char *s, wchar_t wc, mbstate_t *ps) { /* This implementation of wcrtomb on top of wctomb() supports only stateless encodings. ps must be in the initial state. */ if (ps != NULL && !mbsinit (ps)) { errno = EINVAL; return (size_t)(-1); } if (s == NULL) /* We know the NUL wide character corresponds to the NUL character. */ return 1; else { int ret = wctomb (s, wc); if (ret >= 0) return ret; else { errno = EILSEQ; return (size_t)(-1); } } } gnuastro-0.5/bootstrapped/lib/vsnprintf.c0000644000175000017500000000354113217200021015601 00000000000000/* Formatted output to strings. Copyright (C) 2004, 2006-2017 Free Software Foundation, Inc. Written by Simon Josefsson and Yoann Vandoorselaere . This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifdef HAVE_CONFIG_H # include #endif /* Specification. */ #include #include #include #include #include #include #include "vasnprintf.h" /* Print formatted output to string STR. Similar to vsprintf, but additional length SIZE limit how much is written into STR. Returns string length of formatted string (which may be larger than SIZE). STR may be NULL, in which case nothing will be written. On error, return a negative value. */ int vsnprintf (char *str, size_t size, const char *format, va_list args) { char *output; size_t len; size_t lenbuf = size; output = vasnprintf (str, &lenbuf, format, args); len = lenbuf; if (!output) return -1; if (output != str) { if (size) { size_t pruned_len = (len < size ? len : size - 1); memcpy (str, output, pruned_len); str[pruned_len] = '\0'; } free (output); } if (len > INT_MAX) { errno = EOVERFLOW; return -1; } return len; } gnuastro-0.5/bootstrapped/lib/vasnprintf.c0000644000175000017500000066634213217200021015760 00000000000000/* vsprintf with automatic memory allocation. Copyright (C) 1999, 2002-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file can be parametrized with the following macros: VASNPRINTF The name of the function being defined. FCHAR_T The element type of the format string. DCHAR_T The element type of the destination (result) string. FCHAR_T_ONLY_ASCII Set to 1 to enable verification that all characters in the format string are ASCII. MUST be set if FCHAR_T and DCHAR_T are not the same type. DIRECTIVE Structure denoting a format directive. Depends on FCHAR_T. DIRECTIVES Structure denoting the set of format directives of a format string. Depends on FCHAR_T. PRINTF_PARSE Function that parses a format string. Depends on FCHAR_T. DCHAR_CPY memcpy like function for DCHAR_T[] arrays. DCHAR_SET memset like function for DCHAR_T[] arrays. DCHAR_MBSNLEN mbsnlen like function for DCHAR_T[] arrays. SNPRINTF The system's snprintf (or similar) function. This may be either snprintf or swprintf. TCHAR_T The element type of the argument and result string of the said SNPRINTF function. This may be either char or wchar_t. The code exploits that sizeof (TCHAR_T) | sizeof (DCHAR_T) and alignof (TCHAR_T) <= alignof (DCHAR_T). DCHAR_IS_TCHAR Set to 1 if DCHAR_T and TCHAR_T are the same type. DCHAR_CONV_FROM_ENCODING A function to convert from char[] to DCHAR[]. DCHAR_IS_UINT8_T Set to 1 if DCHAR_T is uint8_t. DCHAR_IS_UINT16_T Set to 1 if DCHAR_T is uint16_t. DCHAR_IS_UINT32_T Set to 1 if DCHAR_T is uint32_t. */ /* Tell glibc's to provide a prototype for snprintf(). This must come before because may include , and once has been included, it's too late. */ #ifndef _GNU_SOURCE # define _GNU_SOURCE 1 #endif #ifndef VASNPRINTF # include #endif #ifndef IN_LIBINTL # include #endif /* Specification. */ #ifndef VASNPRINTF # if WIDE_CHAR_VERSION # include "vasnwprintf.h" # else # include "vasnprintf.h" # endif #endif #include /* localeconv() */ #include /* snprintf(), sprintf() */ #include /* abort(), malloc(), realloc(), free() */ #include /* memcpy(), strlen() */ #include /* errno */ #include /* CHAR_BIT */ #include /* DBL_MAX_EXP, LDBL_MAX_EXP */ #if HAVE_NL_LANGINFO # include #endif #ifndef VASNPRINTF # if WIDE_CHAR_VERSION # include "wprintf-parse.h" # else # include "printf-parse.h" # endif #endif /* Checked size_t computations. */ #include "xsize.h" #include "verify.h" #if (NEED_PRINTF_DOUBLE || NEED_PRINTF_LONG_DOUBLE) && !defined IN_LIBINTL # include # include "float+.h" #endif #if (NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE) && !defined IN_LIBINTL # include # include "isnand-nolibm.h" #endif #if (NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE) && !defined IN_LIBINTL # include # include "isnanl-nolibm.h" # include "fpucw.h" #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_DOUBLE) && !defined IN_LIBINTL # include # include "isnand-nolibm.h" # include "printf-frexp.h" #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE) && !defined IN_LIBINTL # include # include "isnanl-nolibm.h" # include "printf-frexpl.h" # include "fpucw.h" #endif #ifndef FALLTHROUGH # if __GNUC__ < 7 # define FALLTHROUGH ((void) 0) # else # define FALLTHROUGH __attribute__ ((__fallthrough__)) # endif #endif /* Default parameters. */ #ifndef VASNPRINTF # if WIDE_CHAR_VERSION # define VASNPRINTF vasnwprintf # define FCHAR_T wchar_t # define DCHAR_T wchar_t # define TCHAR_T wchar_t # define DCHAR_IS_TCHAR 1 # define DIRECTIVE wchar_t_directive # define DIRECTIVES wchar_t_directives # define PRINTF_PARSE wprintf_parse # define DCHAR_CPY wmemcpy # define DCHAR_SET wmemset # else # define VASNPRINTF vasnprintf # define FCHAR_T char # define DCHAR_T char # define TCHAR_T char # define DCHAR_IS_TCHAR 1 # define DIRECTIVE char_directive # define DIRECTIVES char_directives # define PRINTF_PARSE printf_parse # define DCHAR_CPY memcpy # define DCHAR_SET memset # endif #endif #if WIDE_CHAR_VERSION /* TCHAR_T is wchar_t. */ # define USE_SNPRINTF 1 # if HAVE_DECL__SNWPRINTF /* On Windows, the function swprintf() has a different signature than on Unix; we use the function _snwprintf() or - on mingw - snwprintf() instead. The mingw function snwprintf() has fewer bugs than the MSVCRT function _snwprintf(), so prefer that. */ # if defined __MINGW32__ # define SNPRINTF snwprintf # else # define SNPRINTF _snwprintf # define USE_MSVC__SNPRINTF 1 # endif # else /* Unix. */ # define SNPRINTF swprintf # endif #else /* TCHAR_T is char. */ /* Use snprintf if it exists under the name 'snprintf' or '_snprintf'. But don't use it on BeOS, since BeOS snprintf produces no output if the size argument is >= 0x3000000. Also don't use it on Linux libc5, since there snprintf with size = 1 writes any output without bounds, like sprintf. */ # if (HAVE_DECL__SNPRINTF || HAVE_SNPRINTF) && !defined __BEOS__ && !(__GNU_LIBRARY__ == 1) # define USE_SNPRINTF 1 # else # define USE_SNPRINTF 0 # endif # if HAVE_DECL__SNPRINTF /* Windows. The mingw function snprintf() has fewer bugs than the MSVCRT function _snprintf(), so prefer that. */ # if defined __MINGW32__ # define SNPRINTF snprintf /* Here we need to call the native snprintf, not rpl_snprintf. */ # undef snprintf # else /* MSVC versions < 14 did not have snprintf, only _snprintf. */ # define SNPRINTF _snprintf # define USE_MSVC__SNPRINTF 1 # endif # else /* Unix. */ # define SNPRINTF snprintf /* Here we need to call the native snprintf, not rpl_snprintf. */ # undef snprintf # endif #endif /* Here we need to call the native sprintf, not rpl_sprintf. */ #undef sprintf /* GCC >= 4.0 with -Wall emits unjustified "... may be used uninitialized" warnings in this file. Use -Dlint to suppress them. */ #if defined GCC_LINT || defined lint # define IF_LINT(Code) Code #else # define IF_LINT(Code) /* empty */ #endif /* Avoid some warnings from "gcc -Wshadow". This file doesn't use the exp() and remainder() functions. */ #undef exp #define exp expo #undef remainder #define remainder rem #if (!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF) && !WIDE_CHAR_VERSION # if (HAVE_STRNLEN && !defined _AIX) # define local_strnlen strnlen # else # ifndef local_strnlen_defined # define local_strnlen_defined 1 static size_t local_strnlen (const char *string, size_t maxlen) { const char *end = memchr (string, '\0', maxlen); return end ? (size_t) (end - string) : maxlen; } # endif # endif #endif #if (((!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF) && WIDE_CHAR_VERSION) || ((!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF || (NEED_PRINTF_DIRECTIVE_LS && !defined IN_LIBINTL)) && !WIDE_CHAR_VERSION && DCHAR_IS_TCHAR)) && HAVE_WCHAR_T # if HAVE_WCSLEN # define local_wcslen wcslen # else /* Solaris 2.5.1 has wcslen() in a separate library libw.so. To avoid a dependency towards this library, here is a local substitute. Define this substitute only once, even if this file is included twice in the same compilation unit. */ # ifndef local_wcslen_defined # define local_wcslen_defined 1 static size_t local_wcslen (const wchar_t *s) { const wchar_t *ptr; for (ptr = s; *ptr != (wchar_t) 0; ptr++) ; return ptr - s; } # endif # endif #endif #if (!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF) && HAVE_WCHAR_T && WIDE_CHAR_VERSION # if HAVE_WCSNLEN # define local_wcsnlen wcsnlen # else # ifndef local_wcsnlen_defined # define local_wcsnlen_defined 1 static size_t local_wcsnlen (const wchar_t *s, size_t maxlen) { const wchar_t *ptr; for (ptr = s; maxlen > 0 && *ptr != (wchar_t) 0; ptr++, maxlen--) ; return ptr - s; } # endif # endif #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE || NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE) && !defined IN_LIBINTL /* Determine the decimal-point character according to the current locale. */ # ifndef decimal_point_char_defined # define decimal_point_char_defined 1 static char decimal_point_char (void) { const char *point; /* Determine it in a multithread-safe way. We know nl_langinfo is multithread-safe on glibc systems and Mac OS X systems, but is not required to be multithread-safe by POSIX. sprintf(), however, is multithread-safe. localeconv() is rarely multithread-safe. */ # if HAVE_NL_LANGINFO && (__GLIBC__ || defined __UCLIBC__ || (defined __APPLE__ && defined __MACH__)) point = nl_langinfo (RADIXCHAR); # elif 1 char pointbuf[5]; sprintf (pointbuf, "%#.0f", 1.0); point = &pointbuf[1]; # else point = localeconv () -> decimal_point; # endif /* The decimal point is always a single byte: either '.' or ','. */ return (point[0] != '\0' ? point[0] : '.'); } # endif #endif #if NEED_PRINTF_INFINITE_DOUBLE && !NEED_PRINTF_DOUBLE && !defined IN_LIBINTL /* Equivalent to !isfinite(x) || x == 0, but does not require libm. */ static int is_infinite_or_zero (double x) { return isnand (x) || x + x == x; } #endif #if NEED_PRINTF_INFINITE_LONG_DOUBLE && !NEED_PRINTF_LONG_DOUBLE && !defined IN_LIBINTL /* Equivalent to !isfinite(x) || x == 0, but does not require libm. */ static int is_infinite_or_zerol (long double x) { return isnanl (x) || x + x == x; } #endif #if (NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_DOUBLE) && !defined IN_LIBINTL /* Converting 'long double' to decimal without rare rounding bugs requires real bignums. We use the naming conventions of GNU gmp, but vastly simpler (and slower) algorithms. */ typedef unsigned int mp_limb_t; # define GMP_LIMB_BITS 32 verify (sizeof (mp_limb_t) * CHAR_BIT == GMP_LIMB_BITS); typedef unsigned long long mp_twolimb_t; # define GMP_TWOLIMB_BITS 64 verify (sizeof (mp_twolimb_t) * CHAR_BIT == GMP_TWOLIMB_BITS); /* Representation of a bignum >= 0. */ typedef struct { size_t nlimbs; mp_limb_t *limbs; /* Bits in little-endian order, allocated with malloc(). */ } mpn_t; /* Compute the product of two bignums >= 0. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * multiply (mpn_t src1, mpn_t src2, mpn_t *dest) { const mp_limb_t *p1; const mp_limb_t *p2; size_t len1; size_t len2; if (src1.nlimbs <= src2.nlimbs) { len1 = src1.nlimbs; p1 = src1.limbs; len2 = src2.nlimbs; p2 = src2.limbs; } else { len1 = src2.nlimbs; p1 = src2.limbs; len2 = src1.nlimbs; p2 = src1.limbs; } /* Now 0 <= len1 <= len2. */ if (len1 == 0) { /* src1 or src2 is zero. */ dest->nlimbs = 0; dest->limbs = (mp_limb_t *) malloc (1); } else { /* Here 1 <= len1 <= len2. */ size_t dlen; mp_limb_t *dp; size_t k, i, j; dlen = len1 + len2; dp = (mp_limb_t *) malloc (dlen * sizeof (mp_limb_t)); if (dp == NULL) return NULL; for (k = len2; k > 0; ) dp[--k] = 0; for (i = 0; i < len1; i++) { mp_limb_t digit1 = p1[i]; mp_twolimb_t carry = 0; for (j = 0; j < len2; j++) { mp_limb_t digit2 = p2[j]; carry += (mp_twolimb_t) digit1 * (mp_twolimb_t) digit2; carry += dp[i + j]; dp[i + j] = (mp_limb_t) carry; carry = carry >> GMP_LIMB_BITS; } dp[i + len2] = (mp_limb_t) carry; } /* Normalise. */ while (dlen > 0 && dp[dlen - 1] == 0) dlen--; dest->nlimbs = dlen; dest->limbs = dp; } return dest->limbs; } /* Compute the quotient of a bignum a >= 0 and a bignum b > 0. a is written as a = q * b + r with 0 <= r < b. q is the quotient, r the remainder. Finally, round-to-even is performed: If r > b/2 or if r = b/2 and q is odd, q is incremented. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * divide (mpn_t a, mpn_t b, mpn_t *q) { /* Algorithm: First normalise a and b: a=[a[m-1],...,a[0]], b=[b[n-1],...,b[0]] with m>=0 and n>0 (in base beta = 2^GMP_LIMB_BITS). If m=n=1, perform a single-precision division: r:=0, j:=m, while j>0 do {Here (q[m-1]*beta^(m-1)+...+q[j]*beta^j) * b[0] + r*beta^j = = a[m-1]*beta^(m-1)+...+a[j]*beta^j und 0<=r=n>1, perform a multiple-precision division: We have a/b < beta^(m-n+1). s:=intDsize-1-(highest bit in b[n-1]), 0<=s=beta/2. For j=m-n,...,0: {Here 0 <= r < b*beta^(j+1).} Compute q* : q* := floor((r[j+n]*beta+r[j+n-1])/b[n-1]). In case of overflow (q* >= beta) set q* := beta-1. Compute c2 := ((r[j+n]*beta+r[j+n-1]) - q* * b[n-1])*beta + r[j+n-2] and c3 := b[n-2] * q*. {We have 0 <= c2 < 2*beta^2, even 0 <= c2 < beta^2 if no overflow occurred. Furthermore 0 <= c3 < beta^2. If there was overflow and r[j+n]*beta+r[j+n-1] - q* * b[n-1] >= beta, i.e. c2 >= beta^2, the next test can be skipped.} While c3 > c2, {Here 0 <= c2 < c3 < beta^2} Put q* := q* - 1, c2 := c2 + b[n-1]*beta, c3 := c3 - b[n-2]. If q* > 0: Put r := r - b * q* * beta^j. In detail: [r[n+j],...,r[j]] := [r[n+j],...,r[j]] - q* * [b[n-1],...,b[0]]. hence: u:=0, for i:=0 to n-1 do u := u + q* * b[i], r[j+i]:=r[j+i]-(u mod beta) (+ beta, if carry), u:=u div beta (+ 1, if carry in subtraction) r[n+j]:=r[n+j]-u. {Since always u = (q* * [b[i-1],...,b[0]] div beta^i) + 1 < q* + 1 <= beta, the carry u does not overflow.} If a negative carry occurs, put q* := q* - 1 and [r[n+j],...,r[j]] := [r[n+j],...,r[j]] + [0,b[n-1],...,b[0]]. Set q[j] := q*. Normalise [q[m-n],..,q[0]]; this yields the quotient q. Shift [r[n-1],...,r[0]] right by s bits and normalise; this yields the rest r. The room for q[j] can be allocated at the memory location of r[n+j]. Finally, round-to-even: Shift r left by 1 bit. If r > b or if r = b and q[0] is odd, q := q+1. */ const mp_limb_t *a_ptr = a.limbs; size_t a_len = a.nlimbs; const mp_limb_t *b_ptr = b.limbs; size_t b_len = b.nlimbs; mp_limb_t *roomptr; mp_limb_t *tmp_roomptr = NULL; mp_limb_t *q_ptr; size_t q_len; mp_limb_t *r_ptr; size_t r_len; /* Allocate room for a_len+2 digits. (Need a_len+1 digits for the real division and 1 more digit for the final rounding of q.) */ roomptr = (mp_limb_t *) malloc ((a_len + 2) * sizeof (mp_limb_t)); if (roomptr == NULL) return NULL; /* Normalise a. */ while (a_len > 0 && a_ptr[a_len - 1] == 0) a_len--; /* Normalise b. */ for (;;) { if (b_len == 0) /* Division by zero. */ abort (); if (b_ptr[b_len - 1] == 0) b_len--; else break; } /* Here m = a_len >= 0 and n = b_len > 0. */ if (a_len < b_len) { /* m beta^(m-2) <= a/b < beta^m */ r_ptr = roomptr; q_ptr = roomptr + 1; { mp_limb_t den = b_ptr[0]; mp_limb_t remainder = 0; const mp_limb_t *sourceptr = a_ptr + a_len; mp_limb_t *destptr = q_ptr + a_len; size_t count; for (count = a_len; count > 0; count--) { mp_twolimb_t num = ((mp_twolimb_t) remainder << GMP_LIMB_BITS) | *--sourceptr; *--destptr = num / den; remainder = num % den; } /* Normalise and store r. */ if (remainder > 0) { r_ptr[0] = remainder; r_len = 1; } else r_len = 0; /* Normalise q. */ q_len = a_len; if (q_ptr[q_len - 1] == 0) q_len--; } } else { /* n>1: multiple precision division. beta^(m-1) <= a < beta^m, beta^(n-1) <= b < beta^n ==> beta^(m-n-1) <= a/b < beta^(m-n+1). */ /* Determine s. */ size_t s; { mp_limb_t msd = b_ptr[b_len - 1]; /* = b[n-1], > 0 */ /* Determine s = GMP_LIMB_BITS - integer_length (msd). Code copied from gnulib's integer_length.c. */ # if __GNUC__ > 3 || (__GNUC__ == 3 && __GNUC_MINOR__ >= 4) s = __builtin_clz (msd); # else # if defined DBL_EXPBIT0_WORD && defined DBL_EXPBIT0_BIT if (GMP_LIMB_BITS <= DBL_MANT_BIT) { /* Use 'double' operations. Assumes an IEEE 754 'double' implementation. */ # define DBL_EXP_MASK ((DBL_MAX_EXP - DBL_MIN_EXP) | 7) # define DBL_EXP_BIAS (DBL_EXP_MASK / 2 - 1) # define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) union { double value; unsigned int word[NWORDS]; } m; /* Use a single integer to floating-point conversion. */ m.value = msd; s = GMP_LIMB_BITS - (((m.word[DBL_EXPBIT0_WORD] >> DBL_EXPBIT0_BIT) & DBL_EXP_MASK) - DBL_EXP_BIAS); } else # undef NWORDS # endif { s = 31; if (msd >= 0x10000) { msd = msd >> 16; s -= 16; } if (msd >= 0x100) { msd = msd >> 8; s -= 8; } if (msd >= 0x10) { msd = msd >> 4; s -= 4; } if (msd >= 0x4) { msd = msd >> 2; s -= 2; } if (msd >= 0x2) { msd = msd >> 1; s -= 1; } } # endif } /* 0 <= s < GMP_LIMB_BITS. Copy b, shifting it left by s bits. */ if (s > 0) { tmp_roomptr = (mp_limb_t *) malloc (b_len * sizeof (mp_limb_t)); if (tmp_roomptr == NULL) { free (roomptr); return NULL; } { const mp_limb_t *sourceptr = b_ptr; mp_limb_t *destptr = tmp_roomptr; mp_twolimb_t accu = 0; size_t count; for (count = b_len; count > 0; count--) { accu += (mp_twolimb_t) *sourceptr++ << s; *destptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } /* accu must be zero, since that was how s was determined. */ if (accu != 0) abort (); } b_ptr = tmp_roomptr; } /* Copy a, shifting it left by s bits, yields r. Memory layout: At the beginning: r = roomptr[0..a_len], at the end: r = roomptr[0..b_len-1], q = roomptr[b_len..a_len] */ r_ptr = roomptr; if (s == 0) { memcpy (r_ptr, a_ptr, a_len * sizeof (mp_limb_t)); r_ptr[a_len] = 0; } else { const mp_limb_t *sourceptr = a_ptr; mp_limb_t *destptr = r_ptr; mp_twolimb_t accu = 0; size_t count; for (count = a_len; count > 0; count--) { accu += (mp_twolimb_t) *sourceptr++ << s; *destptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } *destptr++ = (mp_limb_t) accu; } q_ptr = roomptr + b_len; q_len = a_len - b_len + 1; /* q will have m-n+1 limbs */ { size_t j = a_len - b_len; /* m-n */ mp_limb_t b_msd = b_ptr[b_len - 1]; /* b[n-1] */ mp_limb_t b_2msd = b_ptr[b_len - 2]; /* b[n-2] */ mp_twolimb_t b_msdd = /* b[n-1]*beta+b[n-2] */ ((mp_twolimb_t) b_msd << GMP_LIMB_BITS) | b_2msd; /* Division loop, traversed m-n+1 times. j counts down, b is unchanged, beta/2 <= b[n-1] < beta. */ for (;;) { mp_limb_t q_star; mp_limb_t c1; if (r_ptr[j + b_len] < b_msd) /* r[j+n] < b[n-1] ? */ { /* Divide r[j+n]*beta+r[j+n-1] by b[n-1], no overflow. */ mp_twolimb_t num = ((mp_twolimb_t) r_ptr[j + b_len] << GMP_LIMB_BITS) | r_ptr[j + b_len - 1]; q_star = num / b_msd; c1 = num % b_msd; } else { /* Overflow, hence r[j+n]*beta+r[j+n-1] >= beta*b[n-1]. */ q_star = (mp_limb_t)~(mp_limb_t)0; /* q* = beta-1 */ /* Test whether r[j+n]*beta+r[j+n-1] - (beta-1)*b[n-1] >= beta <==> r[j+n]*beta+r[j+n-1] + b[n-1] >= beta*b[n-1]+beta <==> b[n-1] < floor((r[j+n]*beta+r[j+n-1]+b[n-1])/beta) {<= beta !}. If yes, jump directly to the subtraction loop. (Otherwise, r[j+n]*beta+r[j+n-1] - (beta-1)*b[n-1] < beta <==> floor((r[j+n]*beta+r[j+n-1]+b[n-1])/beta) = b[n-1] ) */ if (r_ptr[j + b_len] > b_msd || (c1 = r_ptr[j + b_len - 1] + b_msd) < b_msd) /* r[j+n] >= b[n-1]+1 or r[j+n] = b[n-1] and the addition r[j+n-1]+b[n-1] gives a carry. */ goto subtract; } /* q_star = q*, c1 = (r[j+n]*beta+r[j+n-1]) - q* * b[n-1] (>=0, 0, decrease it by b[n-1]*beta+b[n-2]. Because of b[n-1]*beta+b[n-2] >= beta^2/2 this can happen only twice. */ if (c3 > c2) { q_star = q_star - 1; /* q* := q* - 1 */ if (c3 - c2 > b_msdd) q_star = q_star - 1; /* q* := q* - 1 */ } } if (q_star > 0) subtract: { /* Subtract r := r - b * q* * beta^j. */ mp_limb_t cr; { const mp_limb_t *sourceptr = b_ptr; mp_limb_t *destptr = r_ptr + j; mp_twolimb_t carry = 0; size_t count; for (count = b_len; count > 0; count--) { /* Here 0 <= carry <= q*. */ carry = carry + (mp_twolimb_t) q_star * (mp_twolimb_t) *sourceptr++ + (mp_limb_t) ~(*destptr); /* Here 0 <= carry <= beta*q* + beta-1. */ *destptr++ = ~(mp_limb_t) carry; carry = carry >> GMP_LIMB_BITS; /* <= q* */ } cr = (mp_limb_t) carry; } /* Subtract cr from r_ptr[j + b_len], then forget about r_ptr[j + b_len]. */ if (cr > r_ptr[j + b_len]) { /* Subtraction gave a carry. */ q_star = q_star - 1; /* q* := q* - 1 */ /* Add b back. */ { const mp_limb_t *sourceptr = b_ptr; mp_limb_t *destptr = r_ptr + j; mp_limb_t carry = 0; size_t count; for (count = b_len; count > 0; count--) { mp_limb_t source1 = *sourceptr++; mp_limb_t source2 = *destptr; *destptr++ = source1 + source2 + carry; carry = (carry ? source1 >= (mp_limb_t) ~source2 : source1 > (mp_limb_t) ~source2); } } /* Forget about the carry and about r[j+n]. */ } } /* q* is determined. Store it as q[j]. */ q_ptr[j] = q_star; if (j == 0) break; j--; } } r_len = b_len; /* Normalise q. */ if (q_ptr[q_len - 1] == 0) q_len--; # if 0 /* Not needed here, since we need r only to compare it with b/2, and b is shifted left by s bits. */ /* Shift r right by s bits. */ if (s > 0) { mp_limb_t ptr = r_ptr + r_len; mp_twolimb_t accu = 0; size_t count; for (count = r_len; count > 0; count--) { accu = (mp_twolimb_t) (mp_limb_t) accu << GMP_LIMB_BITS; accu += (mp_twolimb_t) *--ptr << (GMP_LIMB_BITS - s); *ptr = (mp_limb_t) (accu >> GMP_LIMB_BITS); } } # endif /* Normalise r. */ while (r_len > 0 && r_ptr[r_len - 1] == 0) r_len--; } /* Compare r << 1 with b. */ if (r_len > b_len) goto increment_q; { size_t i; for (i = b_len;;) { mp_limb_t r_i = (i <= r_len && i > 0 ? r_ptr[i - 1] >> (GMP_LIMB_BITS - 1) : 0) | (i < r_len ? r_ptr[i] << 1 : 0); mp_limb_t b_i = (i < b_len ? b_ptr[i] : 0); if (r_i > b_i) goto increment_q; if (r_i < b_i) goto keep_q; if (i == 0) break; i--; } } if (q_len > 0 && ((q_ptr[0] & 1) != 0)) /* q is odd. */ increment_q: { size_t i; for (i = 0; i < q_len; i++) if (++(q_ptr[i]) != 0) goto keep_q; q_ptr[q_len++] = 1; } keep_q: if (tmp_roomptr != NULL) free (tmp_roomptr); q->limbs = q_ptr; q->nlimbs = q_len; return roomptr; } /* Convert a bignum a >= 0, multiplied with 10^extra_zeroes, to decimal representation. Destroys the contents of a. Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * convert_to_decimal (mpn_t a, size_t extra_zeroes) { mp_limb_t *a_ptr = a.limbs; size_t a_len = a.nlimbs; /* 0.03345 is slightly larger than log(2)/(9*log(10)). */ size_t c_len = 9 * ((size_t)(a_len * (GMP_LIMB_BITS * 0.03345f)) + 1); char *c_ptr = (char *) malloc (xsum (c_len, extra_zeroes)); if (c_ptr != NULL) { char *d_ptr = c_ptr; for (; extra_zeroes > 0; extra_zeroes--) *d_ptr++ = '0'; while (a_len > 0) { /* Divide a by 10^9, in-place. */ mp_limb_t remainder = 0; mp_limb_t *ptr = a_ptr + a_len; size_t count; for (count = a_len; count > 0; count--) { mp_twolimb_t num = ((mp_twolimb_t) remainder << GMP_LIMB_BITS) | *--ptr; *ptr = num / 1000000000; remainder = num % 1000000000; } /* Store the remainder as 9 decimal digits. */ for (count = 9; count > 0; count--) { *d_ptr++ = '0' + (remainder % 10); remainder = remainder / 10; } /* Normalize a. */ if (a_ptr[a_len - 1] == 0) a_len--; } /* Remove leading zeroes. */ while (d_ptr > c_ptr && d_ptr[-1] == '0') d_ptr--; /* But keep at least one zero. */ if (d_ptr == c_ptr) *d_ptr++ = '0'; /* Terminate the string. */ *d_ptr = '\0'; } return c_ptr; } # if NEED_PRINTF_LONG_DOUBLE /* Assuming x is finite and >= 0: write x as x = 2^e * m, where m is a bignum. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * decode_long_double (long double x, int *ep, mpn_t *mp) { mpn_t m; int exp; long double y; size_t i; /* Allocate memory for result. */ m.nlimbs = (LDBL_MANT_BIT + GMP_LIMB_BITS - 1) / GMP_LIMB_BITS; m.limbs = (mp_limb_t *) malloc (m.nlimbs * sizeof (mp_limb_t)); if (m.limbs == NULL) return NULL; /* Split into exponential part and mantissa. */ y = frexpl (x, &exp); if (!(y >= 0.0L && y < 1.0L)) abort (); /* x = 2^exp * y = 2^(exp - LDBL_MANT_BIT) * (y * 2^LDBL_MANT_BIT), and the latter is an integer. */ /* Convert the mantissa (y * 2^LDBL_MANT_BIT) to a sequence of limbs. I'm not sure whether it's safe to cast a 'long double' value between 2^31 and 2^32 to 'unsigned int', therefore play safe and cast only 'long double' values between 0 and 2^16 (to 'unsigned int' or 'int', doesn't matter). */ # if (LDBL_MANT_BIT % GMP_LIMB_BITS) != 0 # if (LDBL_MANT_BIT % GMP_LIMB_BITS) > GMP_LIMB_BITS / 2 { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (LDBL_MANT_BIT % (GMP_LIMB_BITS / 2)); hi = (int) y; y -= hi; if (!(y >= 0.0L && y < 1.0L)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0L && y < 1.0L)) abort (); m.limbs[LDBL_MANT_BIT / GMP_LIMB_BITS] = (hi << (GMP_LIMB_BITS / 2)) | lo; } # else { mp_limb_t d; y *= (mp_limb_t) 1 << (LDBL_MANT_BIT % GMP_LIMB_BITS); d = (int) y; y -= d; if (!(y >= 0.0L && y < 1.0L)) abort (); m.limbs[LDBL_MANT_BIT / GMP_LIMB_BITS] = d; } # endif # endif for (i = LDBL_MANT_BIT / GMP_LIMB_BITS; i > 0; ) { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); hi = (int) y; y -= hi; if (!(y >= 0.0L && y < 1.0L)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0L && y < 1.0L)) abort (); m.limbs[--i] = (hi << (GMP_LIMB_BITS / 2)) | lo; } # if 0 /* On FreeBSD 6.1/x86, 'long double' numbers sometimes have excess precision. */ if (!(y == 0.0L)) abort (); # endif /* Normalise. */ while (m.nlimbs > 0 && m.limbs[m.nlimbs - 1] == 0) m.nlimbs--; *mp = m; *ep = exp - LDBL_MANT_BIT; return m.limbs; } # endif # if NEED_PRINTF_DOUBLE /* Assuming x is finite and >= 0: write x as x = 2^e * m, where m is a bignum. Return the allocated memory in case of success, NULL in case of memory allocation failure. */ static void * decode_double (double x, int *ep, mpn_t *mp) { mpn_t m; int exp; double y; size_t i; /* Allocate memory for result. */ m.nlimbs = (DBL_MANT_BIT + GMP_LIMB_BITS - 1) / GMP_LIMB_BITS; m.limbs = (mp_limb_t *) malloc (m.nlimbs * sizeof (mp_limb_t)); if (m.limbs == NULL) return NULL; /* Split into exponential part and mantissa. */ y = frexp (x, &exp); if (!(y >= 0.0 && y < 1.0)) abort (); /* x = 2^exp * y = 2^(exp - DBL_MANT_BIT) * (y * 2^DBL_MANT_BIT), and the latter is an integer. */ /* Convert the mantissa (y * 2^DBL_MANT_BIT) to a sequence of limbs. I'm not sure whether it's safe to cast a 'double' value between 2^31 and 2^32 to 'unsigned int', therefore play safe and cast only 'double' values between 0 and 2^16 (to 'unsigned int' or 'int', doesn't matter). */ # if (DBL_MANT_BIT % GMP_LIMB_BITS) != 0 # if (DBL_MANT_BIT % GMP_LIMB_BITS) > GMP_LIMB_BITS / 2 { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (DBL_MANT_BIT % (GMP_LIMB_BITS / 2)); hi = (int) y; y -= hi; if (!(y >= 0.0 && y < 1.0)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0 && y < 1.0)) abort (); m.limbs[DBL_MANT_BIT / GMP_LIMB_BITS] = (hi << (GMP_LIMB_BITS / 2)) | lo; } # else { mp_limb_t d; y *= (mp_limb_t) 1 << (DBL_MANT_BIT % GMP_LIMB_BITS); d = (int) y; y -= d; if (!(y >= 0.0 && y < 1.0)) abort (); m.limbs[DBL_MANT_BIT / GMP_LIMB_BITS] = d; } # endif # endif for (i = DBL_MANT_BIT / GMP_LIMB_BITS; i > 0; ) { mp_limb_t hi, lo; y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); hi = (int) y; y -= hi; if (!(y >= 0.0 && y < 1.0)) abort (); y *= (mp_limb_t) 1 << (GMP_LIMB_BITS / 2); lo = (int) y; y -= lo; if (!(y >= 0.0 && y < 1.0)) abort (); m.limbs[--i] = (hi << (GMP_LIMB_BITS / 2)) | lo; } if (!(y == 0.0)) abort (); /* Normalise. */ while (m.nlimbs > 0 && m.limbs[m.nlimbs - 1] == 0) m.nlimbs--; *mp = m; *ep = exp - DBL_MANT_BIT; return m.limbs; } # endif /* Assuming x = 2^e * m is finite and >= 0, and n is an integer: Returns the decimal representation of round (x * 10^n). Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * scale10_round_decimal_decoded (int e, mpn_t m, void *memory, int n) { int s; size_t extra_zeroes; unsigned int abs_n; unsigned int abs_s; mp_limb_t *pow5_ptr; size_t pow5_len; unsigned int s_limbs; unsigned int s_bits; mpn_t pow5; mpn_t z; void *z_memory; char *digits; if (memory == NULL) return NULL; /* x = 2^e * m, hence y = round (2^e * 10^n * m) = round (2^(e+n) * 5^n * m) = round (2^s * 5^n * m). */ s = e + n; extra_zeroes = 0; /* Factor out a common power of 10 if possible. */ if (s > 0 && n > 0) { extra_zeroes = (s < n ? s : n); s -= extra_zeroes; n -= extra_zeroes; } /* Here y = round (2^s * 5^n * m) * 10^extra_zeroes. Before converting to decimal, we need to compute z = round (2^s * 5^n * m). */ /* Compute 5^|n|, possibly shifted by |s| bits if n and s have the same sign. 2.322 is slightly larger than log(5)/log(2). */ abs_n = (n >= 0 ? n : -n); abs_s = (s >= 0 ? s : -s); pow5_ptr = (mp_limb_t *) malloc (((int)(abs_n * (2.322f / GMP_LIMB_BITS)) + 1 + abs_s / GMP_LIMB_BITS + 1) * sizeof (mp_limb_t)); if (pow5_ptr == NULL) { free (memory); return NULL; } /* Initialize with 1. */ pow5_ptr[0] = 1; pow5_len = 1; /* Multiply with 5^|n|. */ if (abs_n > 0) { static mp_limb_t const small_pow5[13 + 1] = { 1, 5, 25, 125, 625, 3125, 15625, 78125, 390625, 1953125, 9765625, 48828125, 244140625, 1220703125 }; unsigned int n13; for (n13 = 0; n13 <= abs_n; n13 += 13) { mp_limb_t digit1 = small_pow5[n13 + 13 <= abs_n ? 13 : abs_n - n13]; size_t j; mp_twolimb_t carry = 0; for (j = 0; j < pow5_len; j++) { mp_limb_t digit2 = pow5_ptr[j]; carry += (mp_twolimb_t) digit1 * (mp_twolimb_t) digit2; pow5_ptr[j] = (mp_limb_t) carry; carry = carry >> GMP_LIMB_BITS; } if (carry > 0) pow5_ptr[pow5_len++] = (mp_limb_t) carry; } } s_limbs = abs_s / GMP_LIMB_BITS; s_bits = abs_s % GMP_LIMB_BITS; if (n >= 0 ? s >= 0 : s <= 0) { /* Multiply with 2^|s|. */ if (s_bits > 0) { mp_limb_t *ptr = pow5_ptr; mp_twolimb_t accu = 0; size_t count; for (count = pow5_len; count > 0; count--) { accu += (mp_twolimb_t) *ptr << s_bits; *ptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } if (accu > 0) { *ptr = (mp_limb_t) accu; pow5_len++; } } if (s_limbs > 0) { size_t count; for (count = pow5_len; count > 0;) { count--; pow5_ptr[s_limbs + count] = pow5_ptr[count]; } for (count = s_limbs; count > 0;) { count--; pow5_ptr[count] = 0; } pow5_len += s_limbs; } pow5.limbs = pow5_ptr; pow5.nlimbs = pow5_len; if (n >= 0) { /* Multiply m with pow5. No division needed. */ z_memory = multiply (m, pow5, &z); } else { /* Divide m by pow5 and round. */ z_memory = divide (m, pow5, &z); } } else { pow5.limbs = pow5_ptr; pow5.nlimbs = pow5_len; if (n >= 0) { /* n >= 0, s < 0. Multiply m with pow5, then divide by 2^|s|. */ mpn_t numerator; mpn_t denominator; void *tmp_memory; tmp_memory = multiply (m, pow5, &numerator); if (tmp_memory == NULL) { free (pow5_ptr); free (memory); return NULL; } /* Construct 2^|s|. */ { mp_limb_t *ptr = pow5_ptr + pow5_len; size_t i; for (i = 0; i < s_limbs; i++) ptr[i] = 0; ptr[s_limbs] = (mp_limb_t) 1 << s_bits; denominator.limbs = ptr; denominator.nlimbs = s_limbs + 1; } z_memory = divide (numerator, denominator, &z); free (tmp_memory); } else { /* n < 0, s > 0. Multiply m with 2^s, then divide by pow5. */ mpn_t numerator; mp_limb_t *num_ptr; num_ptr = (mp_limb_t *) malloc ((m.nlimbs + s_limbs + 1) * sizeof (mp_limb_t)); if (num_ptr == NULL) { free (pow5_ptr); free (memory); return NULL; } { mp_limb_t *destptr = num_ptr; { size_t i; for (i = 0; i < s_limbs; i++) *destptr++ = 0; } if (s_bits > 0) { const mp_limb_t *sourceptr = m.limbs; mp_twolimb_t accu = 0; size_t count; for (count = m.nlimbs; count > 0; count--) { accu += (mp_twolimb_t) *sourceptr++ << s_bits; *destptr++ = (mp_limb_t) accu; accu = accu >> GMP_LIMB_BITS; } if (accu > 0) *destptr++ = (mp_limb_t) accu; } else { const mp_limb_t *sourceptr = m.limbs; size_t count; for (count = m.nlimbs; count > 0; count--) *destptr++ = *sourceptr++; } numerator.limbs = num_ptr; numerator.nlimbs = destptr - num_ptr; } z_memory = divide (numerator, pow5, &z); free (num_ptr); } } free (pow5_ptr); free (memory); /* Here y = round (x * 10^n) = z * 10^extra_zeroes. */ if (z_memory == NULL) return NULL; digits = convert_to_decimal (z, extra_zeroes); free (z_memory); return digits; } # if NEED_PRINTF_LONG_DOUBLE /* Assuming x is finite and >= 0, and n is an integer: Returns the decimal representation of round (x * 10^n). Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * scale10_round_decimal_long_double (long double x, int n) { int e IF_LINT(= 0); mpn_t m; void *memory = decode_long_double (x, &e, &m); return scale10_round_decimal_decoded (e, m, memory, n); } # endif # if NEED_PRINTF_DOUBLE /* Assuming x is finite and >= 0, and n is an integer: Returns the decimal representation of round (x * 10^n). Return the allocated memory - containing the decimal digits in low-to-high order, terminated with a NUL character - in case of success, NULL in case of memory allocation failure. */ static char * scale10_round_decimal_double (double x, int n) { int e IF_LINT(= 0); mpn_t m; void *memory = decode_double (x, &e, &m); return scale10_round_decimal_decoded (e, m, memory, n); } # endif # if NEED_PRINTF_LONG_DOUBLE /* Assuming x is finite and > 0: Return an approximation for n with 10^n <= x < 10^(n+1). The approximation is usually the right n, but may be off by 1 sometimes. */ static int floorlog10l (long double x) { int exp; long double y; double z; double l; /* Split into exponential part and mantissa. */ y = frexpl (x, &exp); if (!(y >= 0.0L && y < 1.0L)) abort (); if (y == 0.0L) return INT_MIN; if (y < 0.5L) { while (y < (1.0L / (1 << (GMP_LIMB_BITS / 2)) / (1 << (GMP_LIMB_BITS / 2)))) { y *= 1.0L * (1 << (GMP_LIMB_BITS / 2)) * (1 << (GMP_LIMB_BITS / 2)); exp -= GMP_LIMB_BITS; } if (y < (1.0L / (1 << 16))) { y *= 1.0L * (1 << 16); exp -= 16; } if (y < (1.0L / (1 << 8))) { y *= 1.0L * (1 << 8); exp -= 8; } if (y < (1.0L / (1 << 4))) { y *= 1.0L * (1 << 4); exp -= 4; } if (y < (1.0L / (1 << 2))) { y *= 1.0L * (1 << 2); exp -= 2; } if (y < (1.0L / (1 << 1))) { y *= 1.0L * (1 << 1); exp -= 1; } } if (!(y >= 0.5L && y < 1.0L)) abort (); /* Compute an approximation for l = log2(x) = exp + log2(y). */ l = exp; z = y; if (z < 0.70710678118654752444) { z *= 1.4142135623730950488; l -= 0.5; } if (z < 0.8408964152537145431) { z *= 1.1892071150027210667; l -= 0.25; } if (z < 0.91700404320467123175) { z *= 1.0905077326652576592; l -= 0.125; } if (z < 0.9576032806985736469) { z *= 1.0442737824274138403; l -= 0.0625; } /* Now 0.95 <= z <= 1.01. */ z = 1 - z; /* log2(1-z) = 1/log(2) * (- z - z^2/2 - z^3/3 - z^4/4 - ...) Four terms are enough to get an approximation with error < 10^-7. */ l -= 1.4426950408889634074 * z * (1.0 + z * (0.5 + z * ((1.0 / 3) + z * 0.25))); /* Finally multiply with log(2)/log(10), yields an approximation for log10(x). */ l *= 0.30102999566398119523; /* Round down to the next integer. */ return (int) l + (l < 0 ? -1 : 0); } # endif # if NEED_PRINTF_DOUBLE /* Assuming x is finite and > 0: Return an approximation for n with 10^n <= x < 10^(n+1). The approximation is usually the right n, but may be off by 1 sometimes. */ static int floorlog10 (double x) { int exp; double y; double z; double l; /* Split into exponential part and mantissa. */ y = frexp (x, &exp); if (!(y >= 0.0 && y < 1.0)) abort (); if (y == 0.0) return INT_MIN; if (y < 0.5) { while (y < (1.0 / (1 << (GMP_LIMB_BITS / 2)) / (1 << (GMP_LIMB_BITS / 2)))) { y *= 1.0 * (1 << (GMP_LIMB_BITS / 2)) * (1 << (GMP_LIMB_BITS / 2)); exp -= GMP_LIMB_BITS; } if (y < (1.0 / (1 << 16))) { y *= 1.0 * (1 << 16); exp -= 16; } if (y < (1.0 / (1 << 8))) { y *= 1.0 * (1 << 8); exp -= 8; } if (y < (1.0 / (1 << 4))) { y *= 1.0 * (1 << 4); exp -= 4; } if (y < (1.0 / (1 << 2))) { y *= 1.0 * (1 << 2); exp -= 2; } if (y < (1.0 / (1 << 1))) { y *= 1.0 * (1 << 1); exp -= 1; } } if (!(y >= 0.5 && y < 1.0)) abort (); /* Compute an approximation for l = log2(x) = exp + log2(y). */ l = exp; z = y; if (z < 0.70710678118654752444) { z *= 1.4142135623730950488; l -= 0.5; } if (z < 0.8408964152537145431) { z *= 1.1892071150027210667; l -= 0.25; } if (z < 0.91700404320467123175) { z *= 1.0905077326652576592; l -= 0.125; } if (z < 0.9576032806985736469) { z *= 1.0442737824274138403; l -= 0.0625; } /* Now 0.95 <= z <= 1.01. */ z = 1 - z; /* log2(1-z) = 1/log(2) * (- z - z^2/2 - z^3/3 - z^4/4 - ...) Four terms are enough to get an approximation with error < 10^-7. */ l -= 1.4426950408889634074 * z * (1.0 + z * (0.5 + z * ((1.0 / 3) + z * 0.25))); /* Finally multiply with log(2)/log(10), yields an approximation for log10(x). */ l *= 0.30102999566398119523; /* Round down to the next integer. */ return (int) l + (l < 0 ? -1 : 0); } # endif /* Tests whether a string of digits consists of exactly PRECISION zeroes and a single '1' digit. */ static int is_borderline (const char *digits, size_t precision) { for (; precision > 0; precision--, digits++) if (*digits != '0') return 0; if (*digits != '1') return 0; digits++; return *digits == '\0'; } #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF /* Use a different function name, to make it possible that the 'wchar_t' parametrization and the 'char' parametrization get compiled in the same translation unit. */ # if WIDE_CHAR_VERSION # define MAX_ROOM_NEEDED wmax_room_needed # else # define MAX_ROOM_NEEDED max_room_needed # endif /* Returns the number of TCHAR_T units needed as temporary space for the result of sprintf or SNPRINTF of a single conversion directive. */ static size_t MAX_ROOM_NEEDED (const arguments *ap, size_t arg_index, FCHAR_T conversion, arg_type type, int flags, size_t width, int has_precision, size_t precision, int pad_ourselves) { size_t tmp_length; switch (conversion) { case 'd': case 'i': case 'u': # if HAVE_LONG_LONG_INT if (type == TYPE_LONGLONGINT || type == TYPE_ULONGLONGINT) tmp_length = (unsigned int) (sizeof (unsigned long long) * CHAR_BIT * 0.30103 /* binary -> decimal */ ) + 1; /* turn floor into ceil */ else # endif if (type == TYPE_LONGINT || type == TYPE_ULONGINT) tmp_length = (unsigned int) (sizeof (unsigned long) * CHAR_BIT * 0.30103 /* binary -> decimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (sizeof (unsigned int) * CHAR_BIT * 0.30103 /* binary -> decimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Multiply by 2, as an estimate for FLAG_GROUP. */ tmp_length = xsum (tmp_length, tmp_length); /* Add 1, to account for a leading sign. */ tmp_length = xsum (tmp_length, 1); break; case 'o': # if HAVE_LONG_LONG_INT if (type == TYPE_LONGLONGINT || type == TYPE_ULONGLONGINT) tmp_length = (unsigned int) (sizeof (unsigned long long) * CHAR_BIT * 0.333334 /* binary -> octal */ ) + 1; /* turn floor into ceil */ else # endif if (type == TYPE_LONGINT || type == TYPE_ULONGINT) tmp_length = (unsigned int) (sizeof (unsigned long) * CHAR_BIT * 0.333334 /* binary -> octal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (sizeof (unsigned int) * CHAR_BIT * 0.333334 /* binary -> octal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Add 1, to account for a leading sign. */ tmp_length = xsum (tmp_length, 1); break; case 'x': case 'X': # if HAVE_LONG_LONG_INT if (type == TYPE_LONGLONGINT || type == TYPE_ULONGLONGINT) tmp_length = (unsigned int) (sizeof (unsigned long long) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1; /* turn floor into ceil */ else # endif if (type == TYPE_LONGINT || type == TYPE_ULONGINT) tmp_length = (unsigned int) (sizeof (unsigned long) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (sizeof (unsigned int) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Add 2, to account for a leading sign or alternate form. */ tmp_length = xsum (tmp_length, 2); break; case 'f': case 'F': if (type == TYPE_LONGDOUBLE) tmp_length = (unsigned int) (LDBL_MAX_EXP * 0.30103 /* binary -> decimal */ * 2 /* estimate for FLAG_GROUP */ ) + 1 /* turn floor into ceil */ + 10; /* sign, decimal point etc. */ else tmp_length = (unsigned int) (DBL_MAX_EXP * 0.30103 /* binary -> decimal */ * 2 /* estimate for FLAG_GROUP */ ) + 1 /* turn floor into ceil */ + 10; /* sign, decimal point etc. */ tmp_length = xsum (tmp_length, precision); break; case 'e': case 'E': case 'g': case 'G': tmp_length = 12; /* sign, decimal point, exponent etc. */ tmp_length = xsum (tmp_length, precision); break; case 'a': case 'A': if (type == TYPE_LONGDOUBLE) tmp_length = (unsigned int) (LDBL_DIG * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) (DBL_DIG * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Account for sign, decimal point etc. */ tmp_length = xsum (tmp_length, 12); break; case 'c': # if HAVE_WINT_T && !WIDE_CHAR_VERSION if (type == TYPE_WIDE_CHAR) tmp_length = MB_CUR_MAX; else # endif tmp_length = 1; break; case 's': # if HAVE_WCHAR_T if (type == TYPE_WIDE_STRING) { # if WIDE_CHAR_VERSION /* ISO C says about %ls in fwprintf: "If the precision is not specified or is greater than the size of the array, the array shall contain a null wide character." So if there is a precision, we must not use wcslen. */ const wchar_t *arg = ap->arg[arg_index].a.a_wide_string; if (has_precision) tmp_length = local_wcsnlen (arg, precision); else tmp_length = local_wcslen (arg); # else /* ISO C says about %ls in fprintf: "If a precision is specified, no more than that many bytes are written (including shift sequences, if any), and the array shall contain a null wide character if, to equal the multibyte character sequence length given by the precision, the function would need to access a wide character one past the end of the array." So if there is a precision, we must not use wcslen. */ /* This case has already been handled separately in VASNPRINTF. */ abort (); # endif } else # endif { # if WIDE_CHAR_VERSION /* ISO C says about %s in fwprintf: "If the precision is not specified or is greater than the size of the converted array, the converted array shall contain a null wide character." So if there is a precision, we must not use strlen. */ /* This case has already been handled separately in VASNPRINTF. */ abort (); # else /* ISO C says about %s in fprintf: "If the precision is not specified or greater than the size of the array, the array shall contain a null character." So if there is a precision, we must not use strlen. */ const char *arg = ap->arg[arg_index].a.a_string; if (has_precision) tmp_length = local_strnlen (arg, precision); else tmp_length = strlen (arg); # endif } break; case 'p': tmp_length = (unsigned int) (sizeof (void *) * CHAR_BIT * 0.25 /* binary -> hexadecimal */ ) + 1 /* turn floor into ceil */ + 2; /* account for leading 0x */ break; default: abort (); } if (!pad_ourselves) { # if ENABLE_UNISTDIO /* Padding considers the number of characters, therefore the number of elements after padding may be > max (tmp_length, width) but is certainly <= tmp_length + width. */ tmp_length = xsum (tmp_length, width); # else /* Padding considers the number of elements, says POSIX. */ if (tmp_length < width) tmp_length = width; # endif } tmp_length = xsum (tmp_length, 1); /* account for trailing NUL */ return tmp_length; } #endif DCHAR_T * VASNPRINTF (DCHAR_T *resultbuf, size_t *lengthp, const FCHAR_T *format, va_list args) { DIRECTIVES d; arguments a; if (PRINTF_PARSE (format, &d, &a) < 0) /* errno is already set. */ return NULL; #define CLEANUP() \ if (d.dir != d.direct_alloc_dir) \ free (d.dir); \ if (a.arg != a.direct_alloc_arg) \ free (a.arg); if (PRINTF_FETCHARGS (args, &a) < 0) { CLEANUP (); errno = EINVAL; return NULL; } { size_t buf_neededlength; TCHAR_T *buf; TCHAR_T *buf_malloced; const FCHAR_T *cp; size_t i; DIRECTIVE *dp; /* Output string accumulator. */ DCHAR_T *result; size_t allocated; size_t length; /* Allocate a small buffer that will hold a directive passed to sprintf or snprintf. */ buf_neededlength = xsum4 (7, d.max_width_length, d.max_precision_length, 6); #if HAVE_ALLOCA if (buf_neededlength < 4000 / sizeof (TCHAR_T)) { buf = (TCHAR_T *) alloca (buf_neededlength * sizeof (TCHAR_T)); buf_malloced = NULL; } else #endif { size_t buf_memsize = xtimes (buf_neededlength, sizeof (TCHAR_T)); if (size_overflow_p (buf_memsize)) goto out_of_memory_1; buf = (TCHAR_T *) malloc (buf_memsize); if (buf == NULL) goto out_of_memory_1; buf_malloced = buf; } if (resultbuf != NULL) { result = resultbuf; allocated = *lengthp; } else { result = NULL; allocated = 0; } length = 0; /* Invariants: result is either == resultbuf or == NULL or malloc-allocated. If length > 0, then result != NULL. */ /* Ensures that allocated >= needed. Aborts through a jump to out_of_memory if needed is SIZE_MAX or otherwise too big. */ #define ENSURE_ALLOCATION(needed) \ if ((needed) > allocated) \ { \ size_t memory_size; \ DCHAR_T *memory; \ \ allocated = (allocated > 0 ? xtimes (allocated, 2) : 12); \ if ((needed) > allocated) \ allocated = (needed); \ memory_size = xtimes (allocated, sizeof (DCHAR_T)); \ if (size_overflow_p (memory_size)) \ goto out_of_memory; \ if (result == resultbuf || result == NULL) \ memory = (DCHAR_T *) malloc (memory_size); \ else \ memory = (DCHAR_T *) realloc (result, memory_size); \ if (memory == NULL) \ goto out_of_memory; \ if (result == resultbuf && length > 0) \ DCHAR_CPY (memory, result, length); \ result = memory; \ } for (cp = format, i = 0, dp = &d.dir[0]; ; cp = dp->dir_end, i++, dp++) { if (cp != dp->dir_start) { size_t n = dp->dir_start - cp; size_t augmented_length = xsum (length, n); ENSURE_ALLOCATION (augmented_length); /* This copies a piece of FCHAR_T[] into a DCHAR_T[]. Here we need that the format string contains only ASCII characters if FCHAR_T and DCHAR_T are not the same type. */ if (sizeof (FCHAR_T) == sizeof (DCHAR_T)) { DCHAR_CPY (result + length, (const DCHAR_T *) cp, n); length = augmented_length; } else { do result[length++] = *cp++; while (--n > 0); } } if (i == d.count) break; /* Execute a single directive. */ if (dp->conversion == '%') { size_t augmented_length; if (!(dp->arg_index == ARG_NONE)) abort (); augmented_length = xsum (length, 1); ENSURE_ALLOCATION (augmented_length); result[length] = '%'; length = augmented_length; } else { if (!(dp->arg_index != ARG_NONE)) abort (); if (dp->conversion == 'n') { switch (a.arg[dp->arg_index].type) { case TYPE_COUNT_SCHAR_POINTER: *a.arg[dp->arg_index].a.a_count_schar_pointer = length; break; case TYPE_COUNT_SHORT_POINTER: *a.arg[dp->arg_index].a.a_count_short_pointer = length; break; case TYPE_COUNT_INT_POINTER: *a.arg[dp->arg_index].a.a_count_int_pointer = length; break; case TYPE_COUNT_LONGINT_POINTER: *a.arg[dp->arg_index].a.a_count_longint_pointer = length; break; #if HAVE_LONG_LONG_INT case TYPE_COUNT_LONGLONGINT_POINTER: *a.arg[dp->arg_index].a.a_count_longlongint_pointer = length; break; #endif default: abort (); } } #if ENABLE_UNISTDIO /* The unistdio extensions. */ else if (dp->conversion == 'U') { arg_type type = a.arg[dp->arg_index].type; int flags = dp->flags; int has_width; size_t width; int has_precision; size_t precision; has_width = 0; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } has_width = 1; } has_precision = 0; precision = 0; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } switch (type) { case TYPE_U8_STRING: { const uint8_t *arg = a.arg[dp->arg_index].a.a_u8_string; const uint8_t *arg_end; size_t characters; if (has_precision) { /* Use only PRECISION characters, from the left. */ arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count = u8_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of characters. */ arg_end = arg; characters = 0; for (;;) { int count = u8_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + u8_strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_UINT8_T { size_t n = arg_end - arg; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_CPY (result + length, arg, n); length += n; } # else { /* Convert. */ DCHAR_T *converted = result + length; size_t converted_len = allocated - length; # if DCHAR_IS_TCHAR /* Convert from UTF-8 to locale encoding. */ converted = u8_conv_to_encoding (locale_charset (), iconveh_question_mark, arg, arg_end - arg, NULL, converted, &converted_len); # else /* Convert from UTF-8 to UTF-16/UTF-32. */ converted = U8_TO_DCHAR (arg, arg_end - arg, converted, &converted_len); # endif if (converted == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } if (converted != result + length) { ENSURE_ALLOCATION (xsum (length, converted_len)); DCHAR_CPY (result + length, converted, converted_len); free (converted); } length += converted_len; } # endif if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } break; case TYPE_U16_STRING: { const uint16_t *arg = a.arg[dp->arg_index].a.a_u16_string; const uint16_t *arg_end; size_t characters; if (has_precision) { /* Use only PRECISION characters, from the left. */ arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count = u16_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of characters. */ arg_end = arg; characters = 0; for (;;) { int count = u16_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + u16_strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_UINT16_T { size_t n = arg_end - arg; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_CPY (result + length, arg, n); length += n; } # else { /* Convert. */ DCHAR_T *converted = result + length; size_t converted_len = allocated - length; # if DCHAR_IS_TCHAR /* Convert from UTF-16 to locale encoding. */ converted = u16_conv_to_encoding (locale_charset (), iconveh_question_mark, arg, arg_end - arg, NULL, converted, &converted_len); # else /* Convert from UTF-16 to UTF-8/UTF-32. */ converted = U16_TO_DCHAR (arg, arg_end - arg, converted, &converted_len); # endif if (converted == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } if (converted != result + length) { ENSURE_ALLOCATION (xsum (length, converted_len)); DCHAR_CPY (result + length, converted, converted_len); free (converted); } length += converted_len; } # endif if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } break; case TYPE_U32_STRING: { const uint32_t *arg = a.arg[dp->arg_index].a.a_u32_string; const uint32_t *arg_end; size_t characters; if (has_precision) { /* Use only PRECISION characters, from the left. */ arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count = u32_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of characters. */ arg_end = arg; characters = 0; for (;;) { int count = u32_strmblen (arg_end); if (count == 0) break; if (count < 0) { if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + u32_strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_UINT32_T { size_t n = arg_end - arg; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_CPY (result + length, arg, n); length += n; } # else { /* Convert. */ DCHAR_T *converted = result + length; size_t converted_len = allocated - length; # if DCHAR_IS_TCHAR /* Convert from UTF-32 to locale encoding. */ converted = u32_conv_to_encoding (locale_charset (), iconveh_question_mark, arg, arg_end - arg, NULL, converted, &converted_len); # else /* Convert from UTF-32 to UTF-8/UTF-16. */ converted = U32_TO_DCHAR (arg, arg_end - arg, converted, &converted_len); # endif if (converted == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } if (converted != result + length) { ENSURE_ALLOCATION (xsum (length, converted_len)); DCHAR_CPY (result + length, converted, converted_len); free (converted); } length += converted_len; } # endif if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } break; default: abort (); } } #endif #if (!USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF || (NEED_PRINTF_DIRECTIVE_LS && !defined IN_LIBINTL)) && HAVE_WCHAR_T else if (dp->conversion == 's' # if WIDE_CHAR_VERSION && a.arg[dp->arg_index].type != TYPE_WIDE_STRING # else && a.arg[dp->arg_index].type == TYPE_WIDE_STRING # endif ) { /* The normal handling of the 's' directive below requires allocating a temporary buffer. The determination of its length (tmp_length), in the case when a precision is specified, below requires a conversion between a char[] string and a wchar_t[] wide string. It could be done, but we have no guarantee that the implementation of sprintf will use the exactly same algorithm. Without this guarantee, it is possible to have buffer overrun bugs. In order to avoid such bugs, we implement the entire processing of the 's' directive ourselves. */ int flags = dp->flags; int has_width; size_t width; int has_precision; size_t precision; has_width = 0; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } has_width = 1; } has_precision = 0; precision = 6; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } # if WIDE_CHAR_VERSION /* %s in vasnwprintf. See the specification of fwprintf. */ { const char *arg = a.arg[dp->arg_index].a.a_string; const char *arg_end; size_t characters; if (has_precision) { /* Use only as many bytes as needed to produce PRECISION wide characters, from the left. */ # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; for (; precision > 0; precision--) { int count; # if HAVE_MBRTOWC count = mbrlen (arg_end, MB_CUR_MAX, &state); # else count = mblen (arg_end, MB_CUR_MAX); # endif if (count == 0) /* Found the terminating NUL. */ break; if (count < 0) { /* Invalid or incomplete multibyte character. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else if (has_width) { /* Use the entire string, and count the number of wide characters. */ # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; for (;;) { int count; # if HAVE_MBRTOWC count = mbrlen (arg_end, MB_CUR_MAX, &state); # else count = mblen (arg_end, MB_CUR_MAX); # endif if (count == 0) /* Found the terminating NUL. */ break; if (count < 0) { /* Invalid or incomplete multibyte character. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end += count; characters++; } } else { /* Use the entire string. */ arg_end = arg + strlen (arg); /* The number of characters doesn't matter. */ characters = 0; } if (characters < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } if (has_precision || has_width) { /* We know the number of wide characters in advance. */ size_t remaining; # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif ENSURE_ALLOCATION (xsum (length, characters)); for (remaining = characters; remaining > 0; remaining--) { wchar_t wc; int count; # if HAVE_MBRTOWC count = mbrtowc (&wc, arg, arg_end - arg, &state); # else count = mbtowc (&wc, arg, arg_end - arg); # endif if (count <= 0) /* mbrtowc not consistent with mbrlen, or mbtowc not consistent with mblen. */ abort (); result[length++] = wc; arg += count; } if (!(arg == arg_end)) abort (); } else { # if HAVE_MBRTOWC mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif while (arg < arg_end) { wchar_t wc; int count; # if HAVE_MBRTOWC count = mbrtowc (&wc, arg, arg_end - arg, &state); # else count = mbtowc (&wc, arg, arg_end - arg); # endif if (count <= 0) /* mbrtowc not consistent with mbrlen, or mbtowc not consistent with mblen. */ abort (); ENSURE_ALLOCATION (xsum (length, 1)); result[length++] = wc; arg += count; } } if (characters < width && (dp->flags & FLAG_LEFT)) { size_t n = width - characters; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } # else /* %ls in vasnprintf. See the specification of fprintf. */ { const wchar_t *arg = a.arg[dp->arg_index].a.a_wide_string; const wchar_t *arg_end; size_t characters; # if !DCHAR_IS_TCHAR /* This code assumes that TCHAR_T is 'char'. */ verify (sizeof (TCHAR_T) == 1); TCHAR_T *tmpsrc; DCHAR_T *tmpdst; size_t tmpdst_len; # endif size_t w; if (has_precision) { /* Use only as many wide characters as needed to produce at most PRECISION bytes, from the left. */ # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; while (precision > 0) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg_end == 0) /* Found the terminating null wide character. */ break; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg_end, &state); # else count = wctomb (cbuf, *arg_end); # endif if (count < 0) { /* Cannot convert. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } if (precision < count) break; arg_end++; characters += count; precision -= count; } } # if DCHAR_IS_TCHAR else if (has_width) # else else # endif { /* Use the entire string, and count the number of bytes. */ # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif arg_end = arg; characters = 0; for (;;) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg_end == 0) /* Found the terminating null wide character. */ break; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg_end, &state); # else count = wctomb (cbuf, *arg_end); # endif if (count < 0) { /* Cannot convert. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } arg_end++; characters += count; } } # if DCHAR_IS_TCHAR else { /* Use the entire string. */ arg_end = arg + local_wcslen (arg); /* The number of bytes doesn't matter. */ characters = 0; } # endif # if !DCHAR_IS_TCHAR /* Convert the string into a piece of temporary memory. */ tmpsrc = (TCHAR_T *) malloc (characters * sizeof (TCHAR_T)); if (tmpsrc == NULL) goto out_of_memory; { TCHAR_T *tmpptr = tmpsrc; size_t remaining; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif for (remaining = characters; remaining > 0; ) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg == 0) abort (); # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg, &state); # else count = wctomb (cbuf, *arg); # endif if (count <= 0) /* Inconsistency. */ abort (); memcpy (tmpptr, cbuf, count); tmpptr += count; arg++; remaining -= count; } if (!(arg == arg_end)) abort (); } /* Convert from TCHAR_T[] to DCHAR_T[]. */ tmpdst = DCHAR_CONV_FROM_ENCODING (locale_charset (), iconveh_question_mark, tmpsrc, characters, NULL, NULL, &tmpdst_len); if (tmpdst == NULL) { int saved_errno = errno; free (tmpsrc); if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } free (tmpsrc); # endif if (has_width) { # if ENABLE_UNISTDIO /* Outside POSIX, it's preferable to compare the width against the number of _characters_ of the converted value. */ w = DCHAR_MBSNLEN (result + length, characters); # else /* The width is compared against the number of _bytes_ of the converted value, says POSIX. */ w = characters; # endif } else /* w doesn't matter. */ w = 0; if (w < width && !(dp->flags & FLAG_LEFT)) { size_t n = width - w; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } # if DCHAR_IS_TCHAR if (has_precision || has_width) { /* We know the number of bytes in advance. */ size_t remaining; # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif ENSURE_ALLOCATION (xsum (length, characters)); for (remaining = characters; remaining > 0; ) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg == 0) abort (); # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg, &state); # else count = wctomb (cbuf, *arg); # endif if (count <= 0) /* Inconsistency. */ abort (); memcpy (result + length, cbuf, count); length += count; arg++; remaining -= count; } if (!(arg == arg_end)) abort (); } else { # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t mbstate_t state; memset (&state, '\0', sizeof (mbstate_t)); # endif while (arg < arg_end) { char cbuf[64]; /* Assume MB_CUR_MAX <= 64. */ int count; if (*arg == 0) abort (); # if HAVE_WCRTOMB && !defined GNULIB_defined_mbstate_t count = wcrtomb (cbuf, *arg, &state); # else count = wctomb (cbuf, *arg); # endif if (count <= 0) { /* Cannot convert. */ if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EILSEQ; return NULL; } ENSURE_ALLOCATION (xsum (length, count)); memcpy (result + length, cbuf, count); length += count; arg++; } } # else ENSURE_ALLOCATION (xsum (length, tmpdst_len)); DCHAR_CPY (result + length, tmpdst, tmpdst_len); free (tmpdst); length += tmpdst_len; # endif if (w < width && (dp->flags & FLAG_LEFT)) { size_t n = width - w; ENSURE_ALLOCATION (xsum (length, n)); DCHAR_SET (result + length, ' ', n); length += n; } } # endif } #endif #if (NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_DOUBLE) && !defined IN_LIBINTL else if ((dp->conversion == 'a' || dp->conversion == 'A') # if !(NEED_PRINTF_DIRECTIVE_A || (NEED_PRINTF_LONG_DOUBLE && NEED_PRINTF_DOUBLE)) && (0 # if NEED_PRINTF_DOUBLE || a.arg[dp->arg_index].type == TYPE_DOUBLE # endif # if NEED_PRINTF_LONG_DOUBLE || a.arg[dp->arg_index].type == TYPE_LONGDOUBLE # endif ) # endif ) { arg_type type = a.arg[dp->arg_index].type; int flags = dp->flags; size_t width; int has_precision; size_t precision; size_t tmp_length; size_t count; DCHAR_T tmpbuf[700]; DCHAR_T *tmp; DCHAR_T *pad_ptr; DCHAR_T *p; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } } has_precision = 0; precision = 0; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } /* Allocate a temporary buffer of sufficient size. */ if (type == TYPE_LONGDOUBLE) tmp_length = (unsigned int) ((LDBL_DIG + 1) * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ else tmp_length = (unsigned int) ((DBL_DIG + 1) * 0.831 /* decimal -> hexadecimal */ ) + 1; /* turn floor into ceil */ if (tmp_length < precision) tmp_length = precision; /* Account for sign, decimal point etc. */ tmp_length = xsum (tmp_length, 12); if (tmp_length < width) tmp_length = width; tmp_length = xsum (tmp_length, 1); /* account for trailing NUL */ if (tmp_length <= sizeof (tmpbuf) / sizeof (DCHAR_T)) tmp = tmpbuf; else { size_t tmp_memsize = xtimes (tmp_length, sizeof (DCHAR_T)); if (size_overflow_p (tmp_memsize)) /* Overflow, would lead to out of memory. */ goto out_of_memory; tmp = (DCHAR_T *) malloc (tmp_memsize); if (tmp == NULL) /* Out of memory. */ goto out_of_memory; } pad_ptr = NULL; p = tmp; if (type == TYPE_LONGDOUBLE) { # if NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_LONG_DOUBLE long double arg = a.arg[dp->arg_index].a.a_longdouble; if (isnanl (arg)) { if (dp->conversion == 'A') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; DECL_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING (); if (signbit (arg)) /* arg < 0.0L or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0L && arg + arg == arg) { if (dp->conversion == 'A') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { int exponent; long double mantissa; if (arg > 0.0L) mantissa = printf_frexpl (arg, &exponent); else { exponent = 0; mantissa = 0.0L; } if (has_precision && precision < (unsigned int) ((LDBL_DIG + 1) * 0.831) + 1) { /* Round the mantissa. */ long double tail = mantissa; size_t q; for (q = precision; ; q--) { int digit = (int) tail; tail -= digit; if (q == 0) { if (digit & 1 ? tail >= 0.5L : tail > 0.5L) tail = 1 - tail; else tail = - tail; break; } tail *= 16.0L; } if (tail != 0.0L) for (q = precision; q > 0; q--) tail *= 0.0625L; mantissa += tail; } *p++ = '0'; *p++ = dp->conversion - 'A' + 'X'; pad_ptr = p; { int digit; digit = (int) mantissa; mantissa -= digit; *p++ = '0' + digit; if ((flags & FLAG_ALT) || mantissa > 0.0L || precision > 0) { *p++ = decimal_point_char (); /* This loop terminates because we assume that FLT_RADIX is a power of 2. */ while (mantissa > 0.0L) { mantissa *= 16.0L; digit = (int) mantissa; mantissa -= digit; *p++ = digit + (digit < 10 ? '0' : dp->conversion - 10); if (precision > 0) precision--; } while (precision > 0) { *p++ = '0'; precision--; } } } *p++ = dp->conversion - 'A' + 'P'; # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } END_LONG_DOUBLE_ROUNDING (); } # else abort (); # endif } else { # if NEED_PRINTF_DIRECTIVE_A || NEED_PRINTF_DOUBLE double arg = a.arg[dp->arg_index].a.a_double; if (isnand (arg)) { if (dp->conversion == 'A') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; if (signbit (arg)) /* arg < 0.0 or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0 && arg + arg == arg) { if (dp->conversion == 'A') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { int exponent; double mantissa; if (arg > 0.0) mantissa = printf_frexp (arg, &exponent); else { exponent = 0; mantissa = 0.0; } if (has_precision && precision < (unsigned int) ((DBL_DIG + 1) * 0.831) + 1) { /* Round the mantissa. */ double tail = mantissa; size_t q; for (q = precision; ; q--) { int digit = (int) tail; tail -= digit; if (q == 0) { if (digit & 1 ? tail >= 0.5 : tail > 0.5) tail = 1 - tail; else tail = - tail; break; } tail *= 16.0; } if (tail != 0.0) for (q = precision; q > 0; q--) tail *= 0.0625; mantissa += tail; } *p++ = '0'; *p++ = dp->conversion - 'A' + 'X'; pad_ptr = p; { int digit; digit = (int) mantissa; mantissa -= digit; *p++ = '0' + digit; if ((flags & FLAG_ALT) || mantissa > 0.0 || precision > 0) { *p++ = decimal_point_char (); /* This loop terminates because we assume that FLT_RADIX is a power of 2. */ while (mantissa > 0.0) { mantissa *= 16.0; digit = (int) mantissa; mantissa -= digit; *p++ = digit + (digit < 10 ? '0' : dp->conversion - 10); if (precision > 0) precision--; } while (precision > 0) { *p++ = '0'; precision--; } } } *p++ = dp->conversion - 'A' + 'P'; # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } } # else abort (); # endif } /* The generated string now extends from tmp to p, with the zero padding insertion point being at pad_ptr. */ count = p - tmp; if (count < width) { size_t pad = width - count; DCHAR_T *end = p + pad; if (flags & FLAG_LEFT) { /* Pad with spaces on the right. */ for (; pad > 0; pad--) *p++ = ' '; } else if ((flags & FLAG_ZERO) && pad_ptr != NULL) { /* Pad with zeroes. */ DCHAR_T *q = end; while (p > pad_ptr) *--q = *--p; for (; pad > 0; pad--) *p++ = '0'; } else { /* Pad with spaces on the left. */ DCHAR_T *q = end; while (p > tmp) *--q = *--p; for (; pad > 0; pad--) *p++ = ' '; } p = end; } count = p - tmp; if (count >= tmp_length) /* tmp_length was incorrectly calculated - fix the code above! */ abort (); /* Make room for the result. */ if (count >= allocated - length) { size_t n = xsum (length, count); ENSURE_ALLOCATION (n); } /* Append the result. */ memcpy (result + length, tmp, count * sizeof (DCHAR_T)); if (tmp != tmpbuf) free (tmp); length += count; } #endif #if (NEED_PRINTF_INFINITE_DOUBLE || NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE || NEED_PRINTF_LONG_DOUBLE) && !defined IN_LIBINTL else if ((dp->conversion == 'f' || dp->conversion == 'F' || dp->conversion == 'e' || dp->conversion == 'E' || dp->conversion == 'g' || dp->conversion == 'G' || dp->conversion == 'a' || dp->conversion == 'A') && (0 # if NEED_PRINTF_DOUBLE || a.arg[dp->arg_index].type == TYPE_DOUBLE # elif NEED_PRINTF_INFINITE_DOUBLE || (a.arg[dp->arg_index].type == TYPE_DOUBLE /* The systems (mingw) which produce wrong output for Inf, -Inf, and NaN also do so for -0.0. Therefore we treat this case here as well. */ && is_infinite_or_zero (a.arg[dp->arg_index].a.a_double)) # endif # if NEED_PRINTF_LONG_DOUBLE || a.arg[dp->arg_index].type == TYPE_LONGDOUBLE # elif NEED_PRINTF_INFINITE_LONG_DOUBLE || (a.arg[dp->arg_index].type == TYPE_LONGDOUBLE /* Some systems produce wrong output for Inf, -Inf, and NaN. Some systems in this category (IRIX 5.3) also do so for -0.0. Therefore we treat this case here as well. */ && is_infinite_or_zerol (a.arg[dp->arg_index].a.a_longdouble)) # endif )) { # if (NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE) && (NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE) arg_type type = a.arg[dp->arg_index].type; # endif int flags = dp->flags; size_t width; size_t count; int has_precision; size_t precision; size_t tmp_length; DCHAR_T tmpbuf[700]; DCHAR_T *tmp; DCHAR_T *pad_ptr; DCHAR_T *p; width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } } has_precision = 0; precision = 0; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } /* POSIX specifies the default precision to be 6 for %f, %F, %e, %E, but not for %g, %G. Implementations appear to use the same default precision also for %g, %G. But for %a, %A, the default precision is 0. */ if (!has_precision) if (!(dp->conversion == 'a' || dp->conversion == 'A')) precision = 6; /* Allocate a temporary buffer of sufficient size. */ # if NEED_PRINTF_DOUBLE && NEED_PRINTF_LONG_DOUBLE tmp_length = (type == TYPE_LONGDOUBLE ? LDBL_DIG + 1 : DBL_DIG + 1); # elif NEED_PRINTF_INFINITE_DOUBLE && NEED_PRINTF_LONG_DOUBLE tmp_length = (type == TYPE_LONGDOUBLE ? LDBL_DIG + 1 : 0); # elif NEED_PRINTF_LONG_DOUBLE tmp_length = LDBL_DIG + 1; # elif NEED_PRINTF_DOUBLE tmp_length = DBL_DIG + 1; # else tmp_length = 0; # endif if (tmp_length < precision) tmp_length = precision; # if NEED_PRINTF_LONG_DOUBLE # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE if (type == TYPE_LONGDOUBLE) # endif if (dp->conversion == 'f' || dp->conversion == 'F') { long double arg = a.arg[dp->arg_index].a.a_longdouble; if (!(isnanl (arg) || arg + arg == arg)) { /* arg is finite and nonzero. */ int exponent = floorlog10l (arg < 0 ? -arg : arg); if (exponent >= 0 && tmp_length < exponent + precision) tmp_length = exponent + precision; } } # endif # if NEED_PRINTF_DOUBLE # if NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE if (type == TYPE_DOUBLE) # endif if (dp->conversion == 'f' || dp->conversion == 'F') { double arg = a.arg[dp->arg_index].a.a_double; if (!(isnand (arg) || arg + arg == arg)) { /* arg is finite and nonzero. */ int exponent = floorlog10 (arg < 0 ? -arg : arg); if (exponent >= 0 && tmp_length < exponent + precision) tmp_length = exponent + precision; } } # endif /* Account for sign, decimal point etc. */ tmp_length = xsum (tmp_length, 12); if (tmp_length < width) tmp_length = width; tmp_length = xsum (tmp_length, 1); /* account for trailing NUL */ if (tmp_length <= sizeof (tmpbuf) / sizeof (DCHAR_T)) tmp = tmpbuf; else { size_t tmp_memsize = xtimes (tmp_length, sizeof (DCHAR_T)); if (size_overflow_p (tmp_memsize)) /* Overflow, would lead to out of memory. */ goto out_of_memory; tmp = (DCHAR_T *) malloc (tmp_memsize); if (tmp == NULL) /* Out of memory. */ goto out_of_memory; } pad_ptr = NULL; p = tmp; # if NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_INFINITE_LONG_DOUBLE # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE if (type == TYPE_LONGDOUBLE) # endif { long double arg = a.arg[dp->arg_index].a.a_longdouble; if (isnanl (arg)) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; DECL_LONG_DOUBLE_ROUNDING BEGIN_LONG_DOUBLE_ROUNDING (); if (signbit (arg)) /* arg < 0.0L or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0L && arg + arg == arg) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { # if NEED_PRINTF_LONG_DOUBLE pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { char *digits; size_t ndigits; digits = scale10_round_decimal_long_double (arg, precision); if (digits == NULL) { END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } ndigits = strlen (digits); if (ndigits > precision) do { --ndigits; *p++ = digits[ndigits]; } while (ndigits > precision); else *p++ = '0'; /* Here ndigits <= precision. */ if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > ndigits; precision--) *p++ = '0'; while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } else if (dp->conversion == 'e' || dp->conversion == 'E') { int exponent; if (arg == 0.0L) { exponent = 0; *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else { /* arg > 0.0L. */ int adjusted; char *digits; size_t ndigits; exponent = floorlog10l (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_long_double (arg, (int)precision - exponent); if (digits == NULL) { END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } ndigits = strlen (digits); if (ndigits == precision + 1) break; if (ndigits < precision || ndigits > precision + 2) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits == precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision+1. */ if (is_borderline (digits, precision)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_long_double (arg, (int)precision - exponent + 1); if (digits2 == NULL) { free (digits); END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } if (strlen (digits2) == precision + 1) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision+1. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } *p++ = dp->conversion; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', '.', '2', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+.2d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+.2d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } else if (dp->conversion == 'g' || dp->conversion == 'G') { if (precision == 0) precision = 1; /* precision >= 1. */ if (arg == 0.0L) /* The exponent is 0, >= -4, < precision. Use fixed-point notation. */ { size_t ndigits = precision; /* Number of trailing zeroes that have to be dropped. */ size_t nzeroes = (flags & FLAG_ALT ? 0 : precision - 1); --ndigits; *p++ = '0'; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = '0'; } } } else { /* arg > 0.0L. */ int exponent; int adjusted; char *digits; size_t ndigits; size_t nzeroes; exponent = floorlog10l (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_long_double (arg, (int)(precision - 1) - exponent); if (digits == NULL) { END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } ndigits = strlen (digits); if (ndigits == precision) break; if (ndigits < precision - 1 || ndigits > precision + 1) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits < precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision. */ if (is_borderline (digits, precision - 1)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_long_double (arg, (int)(precision - 1) - exponent + 1); if (digits2 == NULL) { free (digits); END_LONG_DOUBLE_ROUNDING (); goto out_of_memory; } if (strlen (digits2) == precision) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision. */ /* Determine the number of trailing zeroes that have to be dropped. */ nzeroes = 0; if ((flags & FLAG_ALT) == 0) while (nzeroes < ndigits && digits[nzeroes] == '0') nzeroes++; /* The exponent is now determined. */ if (exponent >= -4 && exponent < (long)precision) { /* Fixed-point notation: max(exponent,0)+1 digits, then the decimal point, then the remaining digits without trailing zeroes. */ if (exponent >= 0) { size_t ecount = exponent + 1; /* Note: count <= precision = ndigits. */ for (; ecount > 0; ecount--) *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { size_t ecount = -exponent - 1; *p++ = '0'; *p++ = decimal_point_char (); for (; ecount > 0; ecount--) *p++ = '0'; while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { /* Exponential notation. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } *p++ = dp->conversion - 'G' + 'E'; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = { '%', '+', '.', '2', 'd', '\0' }; SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, "%+.2d", exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, "%+.2d", exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } # endif } free (digits); } } else abort (); # else /* arg is finite. */ if (!(arg == 0.0L)) abort (); pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else if (dp->conversion == 'e' || dp->conversion == 'E') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } *p++ = dp->conversion; /* 'e' or 'E' */ *p++ = '+'; *p++ = '0'; *p++ = '0'; } else if (dp->conversion == 'g' || dp->conversion == 'G') { *p++ = '0'; if (flags & FLAG_ALT) { size_t ndigits = (precision > 0 ? precision - 1 : 0); *p++ = decimal_point_char (); for (; ndigits > 0; --ndigits) *p++ = '0'; } } else if (dp->conversion == 'a' || dp->conversion == 'A') { *p++ = '0'; *p++ = dp->conversion - 'A' + 'X'; pad_ptr = p; *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } *p++ = dp->conversion - 'A' + 'P'; *p++ = '+'; *p++ = '0'; } else abort (); # endif } END_LONG_DOUBLE_ROUNDING (); } } # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE else # endif # endif # if NEED_PRINTF_DOUBLE || NEED_PRINTF_INFINITE_DOUBLE { double arg = a.arg[dp->arg_index].a.a_double; if (isnand (arg)) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'N'; *p++ = 'A'; *p++ = 'N'; } else { *p++ = 'n'; *p++ = 'a'; *p++ = 'n'; } } else { int sign = 0; if (signbit (arg)) /* arg < 0.0 or negative zero */ { sign = -1; arg = -arg; } if (sign < 0) *p++ = '-'; else if (flags & FLAG_SHOWSIGN) *p++ = '+'; else if (flags & FLAG_SPACE) *p++ = ' '; if (arg > 0.0 && arg + arg == arg) { if (dp->conversion >= 'A' && dp->conversion <= 'Z') { *p++ = 'I'; *p++ = 'N'; *p++ = 'F'; } else { *p++ = 'i'; *p++ = 'n'; *p++ = 'f'; } } else { # if NEED_PRINTF_DOUBLE pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { char *digits; size_t ndigits; digits = scale10_round_decimal_double (arg, precision); if (digits == NULL) goto out_of_memory; ndigits = strlen (digits); if (ndigits > precision) do { --ndigits; *p++ = digits[ndigits]; } while (ndigits > precision); else *p++ = '0'; /* Here ndigits <= precision. */ if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > ndigits; precision--) *p++ = '0'; while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } else if (dp->conversion == 'e' || dp->conversion == 'E') { int exponent; if (arg == 0.0) { exponent = 0; *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else { /* arg > 0.0. */ int adjusted; char *digits; size_t ndigits; exponent = floorlog10 (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_double (arg, (int)precision - exponent); if (digits == NULL) goto out_of_memory; ndigits = strlen (digits); if (ndigits == precision + 1) break; if (ndigits < precision || ndigits > precision + 2) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits == precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision+1. */ if (is_borderline (digits, precision)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_double (arg, (int)precision - exponent + 1); if (digits2 == NULL) { free (digits); goto out_of_memory; } if (strlen (digits2) == precision + 1) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision+1. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); while (ndigits > 0) { --ndigits; *p++ = digits[ndigits]; } } free (digits); } *p++ = dp->conversion; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { '%', '+', '.', '3', 'd', '\0' }; # else { '%', '+', '.', '2', 'd', '\0' }; # endif SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else { static const char decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ "%+.3d"; # else "%+.2d"; # endif if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, decimal_format, exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, decimal_format, exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } } # endif } else if (dp->conversion == 'g' || dp->conversion == 'G') { if (precision == 0) precision = 1; /* precision >= 1. */ if (arg == 0.0) /* The exponent is 0, >= -4, < precision. Use fixed-point notation. */ { size_t ndigits = precision; /* Number of trailing zeroes that have to be dropped. */ size_t nzeroes = (flags & FLAG_ALT ? 0 : precision - 1); --ndigits; *p++ = '0'; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = '0'; } } } else { /* arg > 0.0. */ int exponent; int adjusted; char *digits; size_t ndigits; size_t nzeroes; exponent = floorlog10 (arg); adjusted = 0; for (;;) { digits = scale10_round_decimal_double (arg, (int)(precision - 1) - exponent); if (digits == NULL) goto out_of_memory; ndigits = strlen (digits); if (ndigits == precision) break; if (ndigits < precision - 1 || ndigits > precision + 1) /* The exponent was not guessed precisely enough. */ abort (); if (adjusted) /* None of two values of exponent is the right one. Prevent an endless loop. */ abort (); free (digits); if (ndigits < precision) exponent -= 1; else exponent += 1; adjusted = 1; } /* Here ndigits = precision. */ if (is_borderline (digits, precision - 1)) { /* Maybe the exponent guess was too high and a smaller exponent can be reached by turning a 10...0 into 9...9x. */ char *digits2 = scale10_round_decimal_double (arg, (int)(precision - 1) - exponent + 1); if (digits2 == NULL) { free (digits); goto out_of_memory; } if (strlen (digits2) == precision) { free (digits); digits = digits2; exponent -= 1; } else free (digits2); } /* Here ndigits = precision. */ /* Determine the number of trailing zeroes that have to be dropped. */ nzeroes = 0; if ((flags & FLAG_ALT) == 0) while (nzeroes < ndigits && digits[nzeroes] == '0') nzeroes++; /* The exponent is now determined. */ if (exponent >= -4 && exponent < (long)precision) { /* Fixed-point notation: max(exponent,0)+1 digits, then the decimal point, then the remaining digits without trailing zeroes. */ if (exponent >= 0) { size_t ecount = exponent + 1; /* Note: ecount <= precision = ndigits. */ for (; ecount > 0; ecount--) *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { size_t ecount = -exponent - 1; *p++ = '0'; *p++ = decimal_point_char (); for (; ecount > 0; ecount--) *p++ = '0'; while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } } else { /* Exponential notation. */ *p++ = digits[--ndigits]; if ((flags & FLAG_ALT) || ndigits > nzeroes) { *p++ = decimal_point_char (); while (ndigits > nzeroes) { --ndigits; *p++ = digits[ndigits]; } } *p++ = dp->conversion - 'G' + 'E'; /* 'e' or 'E' */ # if WIDE_CHAR_VERSION { static const wchar_t decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { '%', '+', '.', '3', 'd', '\0' }; # else { '%', '+', '.', '2', 'd', '\0' }; # endif SNPRINTF (p, 6 + 1, decimal_format, exponent); } while (*p != '\0') p++; # else { static const char decimal_format[] = /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ "%+.3d"; # else "%+.2d"; # endif if (sizeof (DCHAR_T) == 1) { sprintf ((char *) p, decimal_format, exponent); while (*p != '\0') p++; } else { char expbuf[6 + 1]; const char *ep; sprintf (expbuf, decimal_format, exponent); for (ep = expbuf; (*p = *ep) != '\0'; ep++) p++; } } # endif } free (digits); } } else abort (); # else /* arg is finite. */ if (!(arg == 0.0)) abort (); pad_ptr = p; if (dp->conversion == 'f' || dp->conversion == 'F') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } } else if (dp->conversion == 'e' || dp->conversion == 'E') { *p++ = '0'; if ((flags & FLAG_ALT) || precision > 0) { *p++ = decimal_point_char (); for (; precision > 0; precision--) *p++ = '0'; } *p++ = dp->conversion; /* 'e' or 'E' */ *p++ = '+'; /* Produce the same number of exponent digits as the native printf implementation. */ # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ *p++ = '0'; # endif *p++ = '0'; *p++ = '0'; } else if (dp->conversion == 'g' || dp->conversion == 'G') { *p++ = '0'; if (flags & FLAG_ALT) { size_t ndigits = (precision > 0 ? precision - 1 : 0); *p++ = decimal_point_char (); for (; ndigits > 0; --ndigits) *p++ = '0'; } } else abort (); # endif } } } # endif /* The generated string now extends from tmp to p, with the zero padding insertion point being at pad_ptr. */ count = p - tmp; if (count < width) { size_t pad = width - count; DCHAR_T *end = p + pad; if (flags & FLAG_LEFT) { /* Pad with spaces on the right. */ for (; pad > 0; pad--) *p++ = ' '; } else if ((flags & FLAG_ZERO) && pad_ptr != NULL) { /* Pad with zeroes. */ DCHAR_T *q = end; while (p > pad_ptr) *--q = *--p; for (; pad > 0; pad--) *p++ = '0'; } else { /* Pad with spaces on the left. */ DCHAR_T *q = end; while (p > tmp) *--q = *--p; for (; pad > 0; pad--) *p++ = ' '; } p = end; } count = p - tmp; if (count >= tmp_length) /* tmp_length was incorrectly calculated - fix the code above! */ abort (); /* Make room for the result. */ if (count >= allocated - length) { size_t n = xsum (length, count); ENSURE_ALLOCATION (n); } /* Append the result. */ memcpy (result + length, tmp, count * sizeof (DCHAR_T)); if (tmp != tmpbuf) free (tmp); length += count; } #endif else { arg_type type = a.arg[dp->arg_index].type; int flags = dp->flags; #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION int has_width; #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF || !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION size_t width; #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF || NEED_PRINTF_UNBOUNDED_PRECISION int has_precision; size_t precision; #endif #if NEED_PRINTF_UNBOUNDED_PRECISION int prec_ourselves; #else # define prec_ourselves 0 #endif #if NEED_PRINTF_FLAG_LEFTADJUST # define pad_ourselves 1 #elif !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION int pad_ourselves; #else # define pad_ourselves 0 #endif TCHAR_T *fbp; unsigned int prefix_count; int prefixes[2] IF_LINT (= { 0 }); int orig_errno; #if !USE_SNPRINTF size_t tmp_length; TCHAR_T tmpbuf[700]; TCHAR_T *tmp; #endif #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION has_width = 0; #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF || !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION width = 0; if (dp->width_start != dp->width_end) { if (dp->width_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->width_arg_index].a.a_int; width = arg; if (arg < 0) { /* "A negative field width is taken as a '-' flag followed by a positive field width." */ flags |= FLAG_LEFT; width = -width; } } else { const FCHAR_T *digitp = dp->width_start; do width = xsum (xtimes (width, 10), *digitp++ - '0'); while (digitp != dp->width_end); } #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION has_width = 1; #endif } #endif #if !USE_SNPRINTF || !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF || NEED_PRINTF_UNBOUNDED_PRECISION has_precision = 0; precision = 6; if (dp->precision_start != dp->precision_end) { if (dp->precision_arg_index != ARG_NONE) { int arg; if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); arg = a.arg[dp->precision_arg_index].a.a_int; /* "A negative precision is taken as if the precision were omitted." */ if (arg >= 0) { precision = arg; has_precision = 1; } } else { const FCHAR_T *digitp = dp->precision_start + 1; precision = 0; while (digitp != dp->precision_end) precision = xsum (xtimes (precision, 10), *digitp++ - '0'); has_precision = 1; } } #endif /* Decide whether to handle the precision ourselves. */ #if NEED_PRINTF_UNBOUNDED_PRECISION switch (dp->conversion) { case 'd': case 'i': case 'u': case 'o': case 'x': case 'X': case 'p': prec_ourselves = has_precision && (precision > 0); break; default: prec_ourselves = 0; break; } #endif /* Decide whether to perform the padding ourselves. */ #if !NEED_PRINTF_FLAG_LEFTADJUST && (!DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION) switch (dp->conversion) { # if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO /* If we need conversion from TCHAR_T[] to DCHAR_T[], we need to perform the padding after this conversion. Functions with unistdio extensions perform the padding based on character count rather than element count. */ case 'c': case 's': # endif # if NEED_PRINTF_FLAG_ZERO case 'f': case 'F': case 'e': case 'E': case 'g': case 'G': case 'a': case 'A': # endif pad_ourselves = 1; break; default: pad_ourselves = prec_ourselves; break; } #endif #if !USE_SNPRINTF /* Allocate a temporary buffer of sufficient size for calling sprintf. */ tmp_length = MAX_ROOM_NEEDED (&a, dp->arg_index, dp->conversion, type, flags, width, has_precision, precision, pad_ourselves); if (tmp_length <= sizeof (tmpbuf) / sizeof (TCHAR_T)) tmp = tmpbuf; else { size_t tmp_memsize = xtimes (tmp_length, sizeof (TCHAR_T)); if (size_overflow_p (tmp_memsize)) /* Overflow, would lead to out of memory. */ goto out_of_memory; tmp = (TCHAR_T *) malloc (tmp_memsize); if (tmp == NULL) /* Out of memory. */ goto out_of_memory; } #endif /* Construct the format string for calling snprintf or sprintf. */ fbp = buf; *fbp++ = '%'; #if NEED_PRINTF_FLAG_GROUPING /* The underlying implementation doesn't support the ' flag. Produce no grouping characters in this case; this is acceptable because the grouping is locale dependent. */ #else if (flags & FLAG_GROUP) *fbp++ = '\''; #endif if (flags & FLAG_LEFT) *fbp++ = '-'; if (flags & FLAG_SHOWSIGN) *fbp++ = '+'; if (flags & FLAG_SPACE) *fbp++ = ' '; if (flags & FLAG_ALT) *fbp++ = '#'; #if __GLIBC__ >= 2 && !defined __UCLIBC__ if (flags & FLAG_LOCALIZED) *fbp++ = 'I'; #endif if (!pad_ourselves) { if (flags & FLAG_ZERO) *fbp++ = '0'; if (dp->width_start != dp->width_end) { size_t n = dp->width_end - dp->width_start; /* The width specification is known to consist only of standard ASCII characters. */ if (sizeof (FCHAR_T) == sizeof (TCHAR_T)) { memcpy (fbp, dp->width_start, n * sizeof (TCHAR_T)); fbp += n; } else { const FCHAR_T *mp = dp->width_start; do *fbp++ = *mp++; while (--n > 0); } } } if (!prec_ourselves) { if (dp->precision_start != dp->precision_end) { size_t n = dp->precision_end - dp->precision_start; /* The precision specification is known to consist only of standard ASCII characters. */ if (sizeof (FCHAR_T) == sizeof (TCHAR_T)) { memcpy (fbp, dp->precision_start, n * sizeof (TCHAR_T)); fbp += n; } else { const FCHAR_T *mp = dp->precision_start; do *fbp++ = *mp++; while (--n > 0); } } } switch (type) { #if HAVE_LONG_LONG_INT case TYPE_LONGLONGINT: case TYPE_ULONGLONGINT: # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ *fbp++ = 'I'; *fbp++ = '6'; *fbp++ = '4'; break; # else *fbp++ = 'l'; # endif #endif FALLTHROUGH; case TYPE_LONGINT: case TYPE_ULONGINT: #if HAVE_WINT_T case TYPE_WIDE_CHAR: #endif #if HAVE_WCHAR_T case TYPE_WIDE_STRING: #endif *fbp++ = 'l'; break; case TYPE_LONGDOUBLE: *fbp++ = 'L'; break; default: break; } #if NEED_PRINTF_DIRECTIVE_F if (dp->conversion == 'F') *fbp = 'f'; else #endif *fbp = dp->conversion; #if USE_SNPRINTF # if ! (((__GLIBC__ > 2 || (__GLIBC__ == 2 && __GLIBC_MINOR__ >= 3)) \ && !defined __UCLIBC__) \ || (defined __APPLE__ && defined __MACH__) \ || ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__)) fbp[1] = '%'; fbp[2] = 'n'; fbp[3] = '\0'; # else /* On glibc2 systems from glibc >= 2.3 - probably also older ones - we know that snprintf's return value conforms to ISO C 99: the tests gl_SNPRINTF_RETVAL_C99 and gl_SNPRINTF_TRUNCATION_C99 pass. Therefore we can avoid using %n in this situation. On glibc2 systems from 2004-10-18 or newer, the use of %n in format strings in writable memory may crash the program (if compiled with _FORTIFY_SOURCE=2), so we should avoid it in this situation. */ /* On Mac OS X 10.3 or newer, we know that snprintf's return value conforms to ISO C 99: the tests gl_SNPRINTF_RETVAL_C99 and gl_SNPRINTF_TRUNCATION_C99 pass. Therefore we can avoid using %n in this situation. On Mac OS X 10.13 or newer, the use of %n in format strings in writable memory by default crashes the program, so we should avoid it in this situation. */ /* On native Windows systems (such as mingw), we can avoid using %n because: - Although the gl_SNPRINTF_TRUNCATION_C99 test fails, snprintf does not write more than the specified number of bytes. (snprintf (buf, 3, "%d %d", 4567, 89) writes '4', '5', '6' into buf, not '4', '5', '\0'.) - Although the gl_SNPRINTF_RETVAL_C99 test fails, snprintf allows us to recognize the case of an insufficient buffer size: it returns -1 in this case. On native Windows systems (such as mingw) where the OS is Windows Vista, the use of %n in format strings by default crashes the program. See and So we should avoid %n in this situation. */ fbp[1] = '\0'; # endif #else fbp[1] = '\0'; #endif /* Construct the arguments for calling snprintf or sprintf. */ prefix_count = 0; if (!pad_ourselves && dp->width_arg_index != ARG_NONE) { if (!(a.arg[dp->width_arg_index].type == TYPE_INT)) abort (); prefixes[prefix_count++] = a.arg[dp->width_arg_index].a.a_int; } if (!prec_ourselves && dp->precision_arg_index != ARG_NONE) { if (!(a.arg[dp->precision_arg_index].type == TYPE_INT)) abort (); prefixes[prefix_count++] = a.arg[dp->precision_arg_index].a.a_int; } #if USE_SNPRINTF /* The SNPRINTF result is appended after result[0..length]. The latter is an array of DCHAR_T; SNPRINTF appends an array of TCHAR_T to it. This is possible because sizeof (TCHAR_T) divides sizeof (DCHAR_T) and alignof (TCHAR_T) <= alignof (DCHAR_T). */ # define TCHARS_PER_DCHAR (sizeof (DCHAR_T) / sizeof (TCHAR_T)) /* Ensure that maxlen below will be >= 2. Needed on BeOS, where an snprintf() with maxlen==1 acts like sprintf(). */ ENSURE_ALLOCATION (xsum (length, (2 + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR)); /* Prepare checking whether snprintf returns the count via %n. */ *(TCHAR_T *) (result + length) = '\0'; #endif orig_errno = errno; for (;;) { int count = -1; #if USE_SNPRINTF int retcount = 0; size_t maxlen = allocated - length; /* SNPRINTF can fail if its second argument is > INT_MAX. */ if (maxlen > INT_MAX / TCHARS_PER_DCHAR) maxlen = INT_MAX / TCHARS_PER_DCHAR; maxlen = maxlen * TCHARS_PER_DCHAR; # define SNPRINTF_BUF(arg) \ switch (prefix_count) \ { \ case 0: \ retcount = SNPRINTF ((TCHAR_T *) (result + length), \ maxlen, buf, \ arg, &count); \ break; \ case 1: \ retcount = SNPRINTF ((TCHAR_T *) (result + length), \ maxlen, buf, \ prefixes[0], arg, &count); \ break; \ case 2: \ retcount = SNPRINTF ((TCHAR_T *) (result + length), \ maxlen, buf, \ prefixes[0], prefixes[1], arg, \ &count); \ break; \ default: \ abort (); \ } #else # define SNPRINTF_BUF(arg) \ switch (prefix_count) \ { \ case 0: \ count = sprintf (tmp, buf, arg); \ break; \ case 1: \ count = sprintf (tmp, buf, prefixes[0], arg); \ break; \ case 2: \ count = sprintf (tmp, buf, prefixes[0], prefixes[1],\ arg); \ break; \ default: \ abort (); \ } #endif errno = 0; switch (type) { case TYPE_SCHAR: { int arg = a.arg[dp->arg_index].a.a_schar; SNPRINTF_BUF (arg); } break; case TYPE_UCHAR: { unsigned int arg = a.arg[dp->arg_index].a.a_uchar; SNPRINTF_BUF (arg); } break; case TYPE_SHORT: { int arg = a.arg[dp->arg_index].a.a_short; SNPRINTF_BUF (arg); } break; case TYPE_USHORT: { unsigned int arg = a.arg[dp->arg_index].a.a_ushort; SNPRINTF_BUF (arg); } break; case TYPE_INT: { int arg = a.arg[dp->arg_index].a.a_int; SNPRINTF_BUF (arg); } break; case TYPE_UINT: { unsigned int arg = a.arg[dp->arg_index].a.a_uint; SNPRINTF_BUF (arg); } break; case TYPE_LONGINT: { long int arg = a.arg[dp->arg_index].a.a_longint; SNPRINTF_BUF (arg); } break; case TYPE_ULONGINT: { unsigned long int arg = a.arg[dp->arg_index].a.a_ulongint; SNPRINTF_BUF (arg); } break; #if HAVE_LONG_LONG_INT case TYPE_LONGLONGINT: { long long int arg = a.arg[dp->arg_index].a.a_longlongint; SNPRINTF_BUF (arg); } break; case TYPE_ULONGLONGINT: { unsigned long long int arg = a.arg[dp->arg_index].a.a_ulonglongint; SNPRINTF_BUF (arg); } break; #endif case TYPE_DOUBLE: { double arg = a.arg[dp->arg_index].a.a_double; SNPRINTF_BUF (arg); } break; case TYPE_LONGDOUBLE: { long double arg = a.arg[dp->arg_index].a.a_longdouble; SNPRINTF_BUF (arg); } break; case TYPE_CHAR: { int arg = a.arg[dp->arg_index].a.a_char; SNPRINTF_BUF (arg); } break; #if HAVE_WINT_T case TYPE_WIDE_CHAR: { wint_t arg = a.arg[dp->arg_index].a.a_wide_char; SNPRINTF_BUF (arg); } break; #endif case TYPE_STRING: { const char *arg = a.arg[dp->arg_index].a.a_string; SNPRINTF_BUF (arg); } break; #if HAVE_WCHAR_T case TYPE_WIDE_STRING: { const wchar_t *arg = a.arg[dp->arg_index].a.a_wide_string; SNPRINTF_BUF (arg); } break; #endif case TYPE_POINTER: { void *arg = a.arg[dp->arg_index].a.a_pointer; SNPRINTF_BUF (arg); } break; default: abort (); } #if USE_SNPRINTF /* Portability: Not all implementations of snprintf() are ISO C 99 compliant. Determine the number of bytes that snprintf() has produced or would have produced. */ if (count >= 0) { /* Verify that snprintf() has NUL-terminated its result. */ if (count < maxlen && ((TCHAR_T *) (result + length)) [count] != '\0') abort (); /* Portability hack. */ if (retcount > count) count = retcount; } else { /* snprintf() doesn't understand the '%n' directive. */ if (fbp[1] != '\0') { /* Don't use the '%n' directive; instead, look at the snprintf() return value. */ fbp[1] = '\0'; continue; } else { /* Look at the snprintf() return value. */ if (retcount < 0) { # if !HAVE_SNPRINTF_RETVAL_C99 || USE_MSVC__SNPRINTF /* HP-UX 10.20 snprintf() is doubly deficient: It doesn't understand the '%n' directive, *and* it returns -1 (rather than the length that would have been required) when the buffer is too small. But a failure at this point can also come from other reasons than a too small buffer, such as an invalid wide string argument to the %ls directive, or possibly an invalid floating-point argument. */ size_t tmp_length = MAX_ROOM_NEEDED (&a, dp->arg_index, dp->conversion, type, flags, width, has_precision, precision, pad_ourselves); if (maxlen < tmp_length) { /* Make more room. But try to do through this reallocation only once. */ size_t bigger_need = xsum (length, xsum (tmp_length, TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR); /* And always grow proportionally. (There may be several arguments, each needing a little more room than the previous one.) */ size_t bigger_need2 = xsum (xtimes (allocated, 2), 12); if (bigger_need < bigger_need2) bigger_need = bigger_need2; ENSURE_ALLOCATION (bigger_need); continue; } # endif } else count = retcount; } } #endif /* Attempt to handle failure. */ if (count < 0) { /* SNPRINTF or sprintf failed. Save and use the errno that it has set, if any. */ int saved_errno = errno; if (saved_errno == 0) { if (dp->conversion == 'c' || dp->conversion == 's') saved_errno = EILSEQ; else saved_errno = EINVAL; } if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } #if USE_SNPRINTF /* Handle overflow of the allocated buffer. If such an overflow occurs, a C99 compliant snprintf() returns a count >= maxlen. However, a non-compliant snprintf() function returns only count = maxlen - 1. To cover both cases, test whether count >= maxlen - 1. */ if ((unsigned int) count + 1 >= maxlen) { /* If maxlen already has attained its allowed maximum, allocating more memory will not increase maxlen. Instead of looping, bail out. */ if (maxlen == INT_MAX / TCHARS_PER_DCHAR) goto overflow; else { /* Need at least (count + 1) * sizeof (TCHAR_T) bytes. (The +1 is for the trailing NUL.) But ask for (count + 2) * sizeof (TCHAR_T) bytes, so that in the next round, we likely get maxlen > (unsigned int) count + 1 and so we don't get here again. And allocate proportionally, to avoid looping eternally if snprintf() reports a too small count. */ size_t n = xmax (xsum (length, ((unsigned int) count + 2 + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR), xtimes (allocated, 2)); ENSURE_ALLOCATION (n); continue; } } #endif #if NEED_PRINTF_UNBOUNDED_PRECISION if (prec_ourselves) { /* Handle the precision. */ TCHAR_T *prec_ptr = # if USE_SNPRINTF (TCHAR_T *) (result + length); # else tmp; # endif size_t prefix_count; size_t move; prefix_count = 0; /* Put the additional zeroes after the sign. */ if (count >= 1 && (*prec_ptr == '-' || *prec_ptr == '+' || *prec_ptr == ' ')) prefix_count = 1; /* Put the additional zeroes after the 0x prefix if (flags & FLAG_ALT) || (dp->conversion == 'p'). */ else if (count >= 2 && prec_ptr[0] == '0' && (prec_ptr[1] == 'x' || prec_ptr[1] == 'X')) prefix_count = 2; move = count - prefix_count; if (precision > move) { /* Insert zeroes. */ size_t insert = precision - move; TCHAR_T *prec_end; # if USE_SNPRINTF size_t n = xsum (length, (count + insert + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR); length += (count + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR; ENSURE_ALLOCATION (n); length -= (count + TCHARS_PER_DCHAR - 1) / TCHARS_PER_DCHAR; prec_ptr = (TCHAR_T *) (result + length); # endif prec_end = prec_ptr + count; prec_ptr += prefix_count; while (prec_end > prec_ptr) { prec_end--; prec_end[insert] = prec_end[0]; } prec_end += insert; do *--prec_end = '0'; while (prec_end > prec_ptr); count += insert; } } #endif #if !USE_SNPRINTF if (count >= tmp_length) /* tmp_length was incorrectly calculated - fix the code above! */ abort (); #endif #if !DCHAR_IS_TCHAR /* Convert from TCHAR_T[] to DCHAR_T[]. */ if (dp->conversion == 'c' || dp->conversion == 's') { /* type = TYPE_CHAR or TYPE_WIDE_CHAR or TYPE_STRING TYPE_WIDE_STRING. The result string is not certainly ASCII. */ const TCHAR_T *tmpsrc; DCHAR_T *tmpdst; size_t tmpdst_len; /* This code assumes that TCHAR_T is 'char'. */ verify (sizeof (TCHAR_T) == 1); # if USE_SNPRINTF tmpsrc = (TCHAR_T *) (result + length); # else tmpsrc = tmp; # endif tmpdst = DCHAR_CONV_FROM_ENCODING (locale_charset (), iconveh_question_mark, tmpsrc, count, NULL, NULL, &tmpdst_len); if (tmpdst == NULL) { int saved_errno = errno; if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = saved_errno; return NULL; } ENSURE_ALLOCATION (xsum (length, tmpdst_len)); DCHAR_CPY (result + length, tmpdst, tmpdst_len); free (tmpdst); count = tmpdst_len; } else { /* The result string is ASCII. Simple 1:1 conversion. */ # if USE_SNPRINTF /* If sizeof (DCHAR_T) == sizeof (TCHAR_T), it's a no-op conversion, in-place on the array starting at (result + length). */ if (sizeof (DCHAR_T) != sizeof (TCHAR_T)) # endif { const TCHAR_T *tmpsrc; DCHAR_T *tmpdst; size_t n; # if USE_SNPRINTF if (result == resultbuf) { tmpsrc = (TCHAR_T *) (result + length); /* ENSURE_ALLOCATION will not move tmpsrc (because it's part of resultbuf). */ ENSURE_ALLOCATION (xsum (length, count)); } else { /* ENSURE_ALLOCATION will move the array (because it uses realloc(). */ ENSURE_ALLOCATION (xsum (length, count)); tmpsrc = (TCHAR_T *) (result + length); } # else tmpsrc = tmp; ENSURE_ALLOCATION (xsum (length, count)); # endif tmpdst = result + length; /* Copy backwards, because of overlapping. */ tmpsrc += count; tmpdst += count; for (n = count; n > 0; n--) *--tmpdst = *--tmpsrc; } } #endif #if DCHAR_IS_TCHAR && !USE_SNPRINTF /* Make room for the result. */ if (count > allocated - length) { /* Need at least count elements. But allocate proportionally. */ size_t n = xmax (xsum (length, count), xtimes (allocated, 2)); ENSURE_ALLOCATION (n); } #endif /* Here count <= allocated - length. */ /* Perform padding. */ #if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO || NEED_PRINTF_FLAG_LEFTADJUST || NEED_PRINTF_FLAG_ZERO || NEED_PRINTF_UNBOUNDED_PRECISION if (pad_ourselves && has_width) { size_t w; # if ENABLE_UNISTDIO /* Outside POSIX, it's preferable to compare the width against the number of _characters_ of the converted value. */ w = DCHAR_MBSNLEN (result + length, count); # else /* The width is compared against the number of _bytes_ of the converted value, says POSIX. */ w = count; # endif if (w < width) { size_t pad = width - w; /* Make room for the result. */ if (xsum (count, pad) > allocated - length) { /* Need at least count + pad elements. But allocate proportionally. */ size_t n = xmax (xsum3 (length, count, pad), xtimes (allocated, 2)); # if USE_SNPRINTF length += count; ENSURE_ALLOCATION (n); length -= count; # else ENSURE_ALLOCATION (n); # endif } /* Here count + pad <= allocated - length. */ { # if !DCHAR_IS_TCHAR || USE_SNPRINTF DCHAR_T * const rp = result + length; # else DCHAR_T * const rp = tmp; # endif DCHAR_T *p = rp + count; DCHAR_T *end = p + pad; DCHAR_T *pad_ptr; # if !DCHAR_IS_TCHAR || ENABLE_UNISTDIO if (dp->conversion == 'c' || dp->conversion == 's') /* No zero-padding for string directives. */ pad_ptr = NULL; else # endif { pad_ptr = (*rp == '-' ? rp + 1 : rp); /* No zero-padding of "inf" and "nan". */ if ((*pad_ptr >= 'A' && *pad_ptr <= 'Z') || (*pad_ptr >= 'a' && *pad_ptr <= 'z')) pad_ptr = NULL; } /* The generated string now extends from rp to p, with the zero padding insertion point being at pad_ptr. */ count = count + pad; /* = end - rp */ if (flags & FLAG_LEFT) { /* Pad with spaces on the right. */ for (; pad > 0; pad--) *p++ = ' '; } else if ((flags & FLAG_ZERO) && pad_ptr != NULL) { /* Pad with zeroes. */ DCHAR_T *q = end; while (p > pad_ptr) *--q = *--p; for (; pad > 0; pad--) *p++ = '0'; } else { /* Pad with spaces on the left. */ DCHAR_T *q = end; while (p > rp) *--q = *--p; for (; pad > 0; pad--) *p++ = ' '; } } } } #endif /* Here still count <= allocated - length. */ #if !DCHAR_IS_TCHAR || USE_SNPRINTF /* The snprintf() result did fit. */ #else /* Append the sprintf() result. */ memcpy (result + length, tmp, count * sizeof (DCHAR_T)); #endif #if !USE_SNPRINTF if (tmp != tmpbuf) free (tmp); #endif #if NEED_PRINTF_DIRECTIVE_F if (dp->conversion == 'F') { /* Convert the %f result to upper case for %F. */ DCHAR_T *rp = result + length; size_t rc; for (rc = count; rc > 0; rc--, rp++) if (*rp >= 'a' && *rp <= 'z') *rp = *rp - 'a' + 'A'; } #endif length += count; break; } errno = orig_errno; #undef pad_ourselves #undef prec_ourselves } } } /* Add the final NUL. */ ENSURE_ALLOCATION (xsum (length, 1)); result[length] = '\0'; if (result != resultbuf && length + 1 < allocated) { /* Shrink the allocated memory if possible. */ DCHAR_T *memory; memory = (DCHAR_T *) realloc (result, (length + 1) * sizeof (DCHAR_T)); if (memory != NULL) result = memory; } if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); *lengthp = length; /* Note that we can produce a big string of a length > INT_MAX. POSIX says that snprintf() fails with errno = EOVERFLOW in this case, but that's only because snprintf() returns an 'int'. This function does not have this limitation. */ return result; #if USE_SNPRINTF overflow: if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); CLEANUP (); errno = EOVERFLOW; return NULL; #endif out_of_memory: if (!(result == resultbuf || result == NULL)) free (result); if (buf_malloced != NULL) free (buf_malloced); out_of_memory_1: CLEANUP (); errno = ENOMEM; return NULL; } } #undef MAX_ROOM_NEEDED #undef TCHARS_PER_DCHAR #undef SNPRINTF #undef USE_SNPRINTF #undef DCHAR_SET #undef DCHAR_CPY #undef PRINTF_PARSE #undef DIRECTIVES #undef DIRECTIVE #undef DCHAR_IS_TCHAR #undef TCHAR_T #undef DCHAR_T #undef FCHAR_T #undef VASNPRINTF gnuastro-0.5/bootstrapped/lib/printf-parse.c0000644000175000017500000005317213217200021016167 00000000000000/* Formatted output to strings. Copyright (C) 1999-2000, 2002-2003, 2006-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file can be parametrized with the following macros: CHAR_T The element type of the format string. CHAR_T_ONLY_ASCII Set to 1 to enable verification that all characters in the format string are ASCII. DIRECTIVE Structure denoting a format directive. Depends on CHAR_T. DIRECTIVES Structure denoting the set of format directives of a format string. Depends on CHAR_T. PRINTF_PARSE Function that parses a format string. Depends on CHAR_T. STATIC Set to 'static' to declare the function static. ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. */ #ifndef PRINTF_PARSE # include #endif /* Specification. */ #ifndef PRINTF_PARSE # include "printf-parse.h" #endif /* Default parameters. */ #ifndef PRINTF_PARSE # define PRINTF_PARSE printf_parse # define CHAR_T char # define DIRECTIVE char_directive # define DIRECTIVES char_directives #endif /* Get size_t, NULL. */ #include /* Get intmax_t. */ #if defined IN_LIBINTL || defined IN_LIBASPRINTF # if HAVE_STDINT_H_WITH_UINTMAX # include # endif # if HAVE_INTTYPES_H_WITH_UINTMAX # include # endif #else # include #endif /* malloc(), realloc(), free(). */ #include /* memcpy(). */ #include /* errno. */ #include /* Checked size_t computations. */ #include "xsize.h" #if CHAR_T_ONLY_ASCII /* c_isascii(). */ # include "c-ctype.h" #endif #ifdef STATIC STATIC #endif int PRINTF_PARSE (const CHAR_T *format, DIRECTIVES *d, arguments *a) { const CHAR_T *cp = format; /* pointer into format */ size_t arg_posn = 0; /* number of regular arguments consumed */ size_t d_allocated; /* allocated elements of d->dir */ size_t a_allocated; /* allocated elements of a->arg */ size_t max_width_length = 0; size_t max_precision_length = 0; d->count = 0; d_allocated = N_DIRECT_ALLOC_DIRECTIVES; d->dir = d->direct_alloc_dir; a->count = 0; a_allocated = N_DIRECT_ALLOC_ARGUMENTS; a->arg = a->direct_alloc_arg; #define REGISTER_ARG(_index_,_type_) \ { \ size_t n = (_index_); \ if (n >= a_allocated) \ { \ size_t memory_size; \ argument *memory; \ \ a_allocated = xtimes (a_allocated, 2); \ if (a_allocated <= n) \ a_allocated = xsum (n, 1); \ memory_size = xtimes (a_allocated, sizeof (argument)); \ if (size_overflow_p (memory_size)) \ /* Overflow, would lead to out of memory. */ \ goto out_of_memory; \ memory = (argument *) (a->arg != a->direct_alloc_arg \ ? realloc (a->arg, memory_size) \ : malloc (memory_size)); \ if (memory == NULL) \ /* Out of memory. */ \ goto out_of_memory; \ if (a->arg == a->direct_alloc_arg) \ memcpy (memory, a->arg, a->count * sizeof (argument)); \ a->arg = memory; \ } \ while (a->count <= n) \ a->arg[a->count++].type = TYPE_NONE; \ if (a->arg[n].type == TYPE_NONE) \ a->arg[n].type = (_type_); \ else if (a->arg[n].type != (_type_)) \ /* Ambiguous type for positional argument. */ \ goto error; \ } while (*cp != '\0') { CHAR_T c = *cp++; if (c == '%') { size_t arg_index = ARG_NONE; DIRECTIVE *dp = &d->dir[d->count]; /* pointer to next directive */ /* Initialize the next directive. */ dp->dir_start = cp - 1; dp->flags = 0; dp->width_start = NULL; dp->width_end = NULL; dp->width_arg_index = ARG_NONE; dp->precision_start = NULL; dp->precision_end = NULL; dp->precision_arg_index = ARG_NONE; dp->arg_index = ARG_NONE; /* Test for positional argument. */ if (*cp >= '0' && *cp <= '9') { const CHAR_T *np; for (np = cp; *np >= '0' && *np <= '9'; np++) ; if (*np == '$') { size_t n = 0; for (np = cp; *np >= '0' && *np <= '9'; np++) n = xsum (xtimes (n, 10), *np - '0'); if (n == 0) /* Positional argument 0. */ goto error; if (size_overflow_p (n)) /* n too large, would lead to out of memory later. */ goto error; arg_index = n - 1; cp = np + 1; } } /* Read the flags. */ for (;;) { if (*cp == '\'') { dp->flags |= FLAG_GROUP; cp++; } else if (*cp == '-') { dp->flags |= FLAG_LEFT; cp++; } else if (*cp == '+') { dp->flags |= FLAG_SHOWSIGN; cp++; } else if (*cp == ' ') { dp->flags |= FLAG_SPACE; cp++; } else if (*cp == '#') { dp->flags |= FLAG_ALT; cp++; } else if (*cp == '0') { dp->flags |= FLAG_ZERO; cp++; } #if __GLIBC__ >= 2 && !defined __UCLIBC__ else if (*cp == 'I') { dp->flags |= FLAG_LOCALIZED; cp++; } #endif else break; } /* Parse the field width. */ if (*cp == '*') { dp->width_start = cp; cp++; dp->width_end = cp; if (max_width_length < 1) max_width_length = 1; /* Test for positional argument. */ if (*cp >= '0' && *cp <= '9') { const CHAR_T *np; for (np = cp; *np >= '0' && *np <= '9'; np++) ; if (*np == '$') { size_t n = 0; for (np = cp; *np >= '0' && *np <= '9'; np++) n = xsum (xtimes (n, 10), *np - '0'); if (n == 0) /* Positional argument 0. */ goto error; if (size_overflow_p (n)) /* n too large, would lead to out of memory later. */ goto error; dp->width_arg_index = n - 1; cp = np + 1; } } if (dp->width_arg_index == ARG_NONE) { dp->width_arg_index = arg_posn++; if (dp->width_arg_index == ARG_NONE) /* arg_posn wrapped around. */ goto error; } REGISTER_ARG (dp->width_arg_index, TYPE_INT); } else if (*cp >= '0' && *cp <= '9') { size_t width_length; dp->width_start = cp; for (; *cp >= '0' && *cp <= '9'; cp++) ; dp->width_end = cp; width_length = dp->width_end - dp->width_start; if (max_width_length < width_length) max_width_length = width_length; } /* Parse the precision. */ if (*cp == '.') { cp++; if (*cp == '*') { dp->precision_start = cp - 1; cp++; dp->precision_end = cp; if (max_precision_length < 2) max_precision_length = 2; /* Test for positional argument. */ if (*cp >= '0' && *cp <= '9') { const CHAR_T *np; for (np = cp; *np >= '0' && *np <= '9'; np++) ; if (*np == '$') { size_t n = 0; for (np = cp; *np >= '0' && *np <= '9'; np++) n = xsum (xtimes (n, 10), *np - '0'); if (n == 0) /* Positional argument 0. */ goto error; if (size_overflow_p (n)) /* n too large, would lead to out of memory later. */ goto error; dp->precision_arg_index = n - 1; cp = np + 1; } } if (dp->precision_arg_index == ARG_NONE) { dp->precision_arg_index = arg_posn++; if (dp->precision_arg_index == ARG_NONE) /* arg_posn wrapped around. */ goto error; } REGISTER_ARG (dp->precision_arg_index, TYPE_INT); } else { size_t precision_length; dp->precision_start = cp - 1; for (; *cp >= '0' && *cp <= '9'; cp++) ; dp->precision_end = cp; precision_length = dp->precision_end - dp->precision_start; if (max_precision_length < precision_length) max_precision_length = precision_length; } } { arg_type type; /* Parse argument type/size specifiers. */ { int flags = 0; for (;;) { if (*cp == 'h') { flags |= (1 << (flags & 1)); cp++; } else if (*cp == 'L') { flags |= 4; cp++; } else if (*cp == 'l') { flags += 8; cp++; } else if (*cp == 'j') { if (sizeof (intmax_t) > sizeof (long)) { /* intmax_t = long long */ flags += 16; } else if (sizeof (intmax_t) > sizeof (int)) { /* intmax_t = long */ flags += 8; } cp++; } else if (*cp == 'z' || *cp == 'Z') { /* 'z' is standardized in ISO C 99, but glibc uses 'Z' because the warning facility in gcc-2.95.2 understands only 'Z' (see gcc-2.95.2/gcc/c-common.c:1784). */ if (sizeof (size_t) > sizeof (long)) { /* size_t = long long */ flags += 16; } else if (sizeof (size_t) > sizeof (int)) { /* size_t = long */ flags += 8; } cp++; } else if (*cp == 't') { if (sizeof (ptrdiff_t) > sizeof (long)) { /* ptrdiff_t = long long */ flags += 16; } else if (sizeof (ptrdiff_t) > sizeof (int)) { /* ptrdiff_t = long */ flags += 8; } cp++; } #if defined __APPLE__ && defined __MACH__ /* On Mac OS X 10.3, PRIdMAX is defined as "qd". We cannot change it to "lld" because PRIdMAX must also be understood by the system's printf routines. */ else if (*cp == 'q') { if (64 / 8 > sizeof (long)) { /* int64_t = long long */ flags += 16; } else { /* int64_t = long */ flags += 8; } cp++; } #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows, PRIdMAX is defined as "I64d". We cannot change it to "lld" because PRIdMAX must also be understood by the system's printf routines. */ else if (*cp == 'I' && cp[1] == '6' && cp[2] == '4') { if (64 / 8 > sizeof (long)) { /* __int64 = long long */ flags += 16; } else { /* __int64 = long */ flags += 8; } cp += 3; } #endif else break; } /* Read the conversion character. */ c = *cp++; switch (c) { case 'd': case 'i': #if HAVE_LONG_LONG_INT /* If 'long long' exists and is larger than 'long': */ if (flags >= 16 || (flags & 4)) type = TYPE_LONGLONGINT; else #endif /* If 'long long' exists and is the same as 'long', we parse "lld" into TYPE_LONGINT. */ if (flags >= 8) type = TYPE_LONGINT; else if (flags & 2) type = TYPE_SCHAR; else if (flags & 1) type = TYPE_SHORT; else type = TYPE_INT; break; case 'o': case 'u': case 'x': case 'X': #if HAVE_LONG_LONG_INT /* If 'long long' exists and is larger than 'long': */ if (flags >= 16 || (flags & 4)) type = TYPE_ULONGLONGINT; else #endif /* If 'unsigned long long' exists and is the same as 'unsigned long', we parse "llu" into TYPE_ULONGINT. */ if (flags >= 8) type = TYPE_ULONGINT; else if (flags & 2) type = TYPE_UCHAR; else if (flags & 1) type = TYPE_USHORT; else type = TYPE_UINT; break; case 'f': case 'F': case 'e': case 'E': case 'g': case 'G': case 'a': case 'A': if (flags >= 16 || (flags & 4)) type = TYPE_LONGDOUBLE; else type = TYPE_DOUBLE; break; case 'c': if (flags >= 8) #if HAVE_WINT_T type = TYPE_WIDE_CHAR; #else goto error; #endif else type = TYPE_CHAR; break; #if HAVE_WINT_T case 'C': type = TYPE_WIDE_CHAR; c = 'c'; break; #endif case 's': if (flags >= 8) #if HAVE_WCHAR_T type = TYPE_WIDE_STRING; #else goto error; #endif else type = TYPE_STRING; break; #if HAVE_WCHAR_T case 'S': type = TYPE_WIDE_STRING; c = 's'; break; #endif case 'p': type = TYPE_POINTER; break; case 'n': #if HAVE_LONG_LONG_INT /* If 'long long' exists and is larger than 'long': */ if (flags >= 16 || (flags & 4)) type = TYPE_COUNT_LONGLONGINT_POINTER; else #endif /* If 'long long' exists and is the same as 'long', we parse "lln" into TYPE_COUNT_LONGINT_POINTER. */ if (flags >= 8) type = TYPE_COUNT_LONGINT_POINTER; else if (flags & 2) type = TYPE_COUNT_SCHAR_POINTER; else if (flags & 1) type = TYPE_COUNT_SHORT_POINTER; else type = TYPE_COUNT_INT_POINTER; break; #if ENABLE_UNISTDIO /* The unistdio extensions. */ case 'U': if (flags >= 16) type = TYPE_U32_STRING; else if (flags >= 8) type = TYPE_U16_STRING; else type = TYPE_U8_STRING; break; #endif case '%': type = TYPE_NONE; break; default: /* Unknown conversion character. */ goto error; } } if (type != TYPE_NONE) { dp->arg_index = arg_index; if (dp->arg_index == ARG_NONE) { dp->arg_index = arg_posn++; if (dp->arg_index == ARG_NONE) /* arg_posn wrapped around. */ goto error; } REGISTER_ARG (dp->arg_index, type); } dp->conversion = c; dp->dir_end = cp; } d->count++; if (d->count >= d_allocated) { size_t memory_size; DIRECTIVE *memory; d_allocated = xtimes (d_allocated, 2); memory_size = xtimes (d_allocated, sizeof (DIRECTIVE)); if (size_overflow_p (memory_size)) /* Overflow, would lead to out of memory. */ goto out_of_memory; memory = (DIRECTIVE *) (d->dir != d->direct_alloc_dir ? realloc (d->dir, memory_size) : malloc (memory_size)); if (memory == NULL) /* Out of memory. */ goto out_of_memory; if (d->dir == d->direct_alloc_dir) memcpy (memory, d->dir, d->count * sizeof (DIRECTIVE)); d->dir = memory; } } #if CHAR_T_ONLY_ASCII else if (!c_isascii (c)) { /* Non-ASCII character. Not supported. */ goto error; } #endif } d->dir[d->count].dir_start = cp; d->max_width_length = max_width_length; d->max_precision_length = max_precision_length; return 0; error: if (a->arg != a->direct_alloc_arg) free (a->arg); if (d->dir != d->direct_alloc_dir) free (d->dir); errno = EINVAL; return -1; out_of_memory: if (a->arg != a->direct_alloc_arg) free (a->arg); if (d->dir != d->direct_alloc_dir) free (d->dir); errno = ENOMEM; return -1; } #undef PRINTF_PARSE #undef DIRECTIVES #undef DIRECTIVE #undef CHAR_T_ONLY_ASCII #undef CHAR_T gnuastro-0.5/bootstrapped/lib/printf-args.c0000644000175000017500000001463313217200021016010 00000000000000/* Decomposed printf argument list. Copyright (C) 1999, 2002-2003, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* This file can be parametrized with the following macros: ENABLE_UNISTDIO Set to 1 to enable the unistdio extensions. PRINTF_FETCHARGS Name of the function to be defined. STATIC Set to 'static' to declare the function static. */ #ifndef PRINTF_FETCHARGS # include #endif /* Specification. */ #ifndef PRINTF_FETCHARGS # include "printf-args.h" #endif #ifdef STATIC STATIC #endif int PRINTF_FETCHARGS (va_list args, arguments *a) { size_t i; argument *ap; for (i = 0, ap = &a->arg[0]; i < a->count; i++, ap++) switch (ap->type) { case TYPE_SCHAR: ap->a.a_schar = va_arg (args, /*signed char*/ int); break; case TYPE_UCHAR: ap->a.a_uchar = va_arg (args, /*unsigned char*/ int); break; case TYPE_SHORT: ap->a.a_short = va_arg (args, /*short*/ int); break; case TYPE_USHORT: ap->a.a_ushort = va_arg (args, /*unsigned short*/ int); break; case TYPE_INT: ap->a.a_int = va_arg (args, int); break; case TYPE_UINT: ap->a.a_uint = va_arg (args, unsigned int); break; case TYPE_LONGINT: ap->a.a_longint = va_arg (args, long int); break; case TYPE_ULONGINT: ap->a.a_ulongint = va_arg (args, unsigned long int); break; #if HAVE_LONG_LONG_INT case TYPE_LONGLONGINT: ap->a.a_longlongint = va_arg (args, long long int); break; case TYPE_ULONGLONGINT: ap->a.a_ulonglongint = va_arg (args, unsigned long long int); break; #endif case TYPE_DOUBLE: ap->a.a_double = va_arg (args, double); break; case TYPE_LONGDOUBLE: ap->a.a_longdouble = va_arg (args, long double); break; case TYPE_CHAR: ap->a.a_char = va_arg (args, int); break; #if HAVE_WINT_T case TYPE_WIDE_CHAR: /* Although ISO C 99 7.24.1.(2) says that wint_t is "unchanged by default argument promotions", this is not the case in mingw32, where wint_t is 'unsigned short'. */ ap->a.a_wide_char = (sizeof (wint_t) < sizeof (int) ? (wint_t) va_arg (args, int) : va_arg (args, wint_t)); break; #endif case TYPE_STRING: ap->a.a_string = va_arg (args, const char *); /* A null pointer is an invalid argument for "%s", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_string == NULL) ap->a.a_string = "(NULL)"; break; #if HAVE_WCHAR_T case TYPE_WIDE_STRING: ap->a.a_wide_string = va_arg (args, const wchar_t *); /* A null pointer is an invalid argument for "%ls", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_wide_string == NULL) { static const wchar_t wide_null_string[] = { (wchar_t)'(', (wchar_t)'N', (wchar_t)'U', (wchar_t)'L', (wchar_t)'L', (wchar_t)')', (wchar_t)0 }; ap->a.a_wide_string = wide_null_string; } break; #endif case TYPE_POINTER: ap->a.a_pointer = va_arg (args, void *); break; case TYPE_COUNT_SCHAR_POINTER: ap->a.a_count_schar_pointer = va_arg (args, signed char *); break; case TYPE_COUNT_SHORT_POINTER: ap->a.a_count_short_pointer = va_arg (args, short *); break; case TYPE_COUNT_INT_POINTER: ap->a.a_count_int_pointer = va_arg (args, int *); break; case TYPE_COUNT_LONGINT_POINTER: ap->a.a_count_longint_pointer = va_arg (args, long int *); break; #if HAVE_LONG_LONG_INT case TYPE_COUNT_LONGLONGINT_POINTER: ap->a.a_count_longlongint_pointer = va_arg (args, long long int *); break; #endif #if ENABLE_UNISTDIO /* The unistdio extensions. */ case TYPE_U8_STRING: ap->a.a_u8_string = va_arg (args, const uint8_t *); /* A null pointer is an invalid argument for "%U", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_u8_string == NULL) { static const uint8_t u8_null_string[] = { '(', 'N', 'U', 'L', 'L', ')', 0 }; ap->a.a_u8_string = u8_null_string; } break; case TYPE_U16_STRING: ap->a.a_u16_string = va_arg (args, const uint16_t *); /* A null pointer is an invalid argument for "%lU", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_u16_string == NULL) { static const uint16_t u16_null_string[] = { '(', 'N', 'U', 'L', 'L', ')', 0 }; ap->a.a_u16_string = u16_null_string; } break; case TYPE_U32_STRING: ap->a.a_u32_string = va_arg (args, const uint32_t *); /* A null pointer is an invalid argument for "%llU", but in practice it occurs quite frequently in printf statements that produce debug output. Use a fallback in this case. */ if (ap->a.a_u32_string == NULL) { static const uint32_t u32_null_string[] = { '(', 'N', 'U', 'L', 'L', ')', 0 }; ap->a.a_u32_string = u32_null_string; } break; #endif default: /* Unknown type. */ return -1; } return 0; } gnuastro-0.5/bootstrapped/lib/asnprintf.c0000644000175000017500000000204713217200020015553 00000000000000/* Formatted output to strings. Copyright (C) 1999, 2002, 2006, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "vasnprintf.h" #include char * asnprintf (char *resultbuf, size_t *lengthp, const char *format, ...) { va_list args; char *result; va_start (args, format); result = vasnprintf (resultbuf, lengthp, format, args); va_end (args); return result; } gnuastro-0.5/bootstrapped/lib/strtok_r.c0000644000175000017500000000411513217200021015415 00000000000000/* Reentrant string tokenizer. Generic version. Copyright (C) 1991, 1996-1999, 2001, 2004, 2007, 2009-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include #ifdef _LIBC # undef strtok_r # undef __strtok_r #else # define __strtok_r strtok_r # define __rawmemchr strchr #endif /* Parse S into tokens separated by characters in DELIM. If S is NULL, the saved pointer in SAVE_PTR is used as the next starting point. For example: char s[] = "-abc-=-def"; char *sp; x = strtok_r(s, "-", &sp); // x = "abc", sp = "=-def" x = strtok_r(NULL, "-=", &sp); // x = "def", sp = NULL x = strtok_r(NULL, "=", &sp); // x = NULL // s = "abc\0-def\0" */ char * __strtok_r (char *s, const char *delim, char **save_ptr) { char *token; if (s == NULL) s = *save_ptr; /* Scan leading delimiters. */ s += strspn (s, delim); if (*s == '\0') { *save_ptr = s; return NULL; } /* Find the end of the token. */ token = s; s = strpbrk (token, delim); if (s == NULL) /* This token finishes the string. */ *save_ptr = __rawmemchr (token, '\0'); else { /* Terminate the token and make *SAVE_PTR point past it. */ *s = '\0'; *save_ptr = s + 1; } return token; } #ifdef weak_alias libc_hidden_def (__strtok_r) weak_alias (__strtok_r, strtok_r) #endif gnuastro-0.5/bootstrapped/lib/strtod.c0000644000175000017500000002416513217200021015074 00000000000000/* Copyright (C) 1991-1992, 1997, 1999, 2003, 2006, 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include #include #include #include #include "c-ctype.h" #ifndef HAVE_LDEXP_IN_LIBC #define HAVE_LDEXP_IN_LIBC 0 #endif /* Return true if C is a space in the current locale, avoiding problems with signed char and isspace. */ static bool locale_isspace (char c) { unsigned char uc = c; return isspace (uc) != 0; } #if !HAVE_LDEXP_IN_LIBC #define ldexp dummy_ldexp /* A dummy definition that will never be invoked. */ static double ldexp (double x _GL_UNUSED, int exponent _GL_UNUSED) { abort (); return 0.0; } #endif /* Return X * BASE**EXPONENT. Return an extreme value and set errno to ERANGE if underflow or overflow occurs. */ static double scale_radix_exp (double x, int radix, long int exponent) { /* If RADIX == 10, this code is neither precise nor fast; it is merely a straightforward and relatively portable approximation. If N == 2, this code is precise on a radix-2 implementation, albeit perhaps not fast if ldexp is not in libc. */ long int e = exponent; if (HAVE_LDEXP_IN_LIBC && radix == 2) return ldexp (x, e < INT_MIN ? INT_MIN : INT_MAX < e ? INT_MAX : e); else { double r = x; if (r != 0) { if (e < 0) { while (e++ != 0) { r /= radix; if (r == 0 && x != 0) { errno = ERANGE; break; } } } else { while (e-- != 0) { if (r < -DBL_MAX / radix) { errno = ERANGE; return -HUGE_VAL; } else if (DBL_MAX / radix < r) { errno = ERANGE; return HUGE_VAL; } else r *= radix; } } } return r; } } /* Parse a number at NPTR; this is a bit like strtol (NPTR, ENDPTR) except there are no leading spaces or signs or "0x", and ENDPTR is nonnull. The number uses a base BASE (either 10 or 16) fraction, a radix RADIX (either 10 or 2) exponent, and exponent character EXPCHAR. To convert from a number of digits to a radix exponent, multiply by RADIX_MULTIPLIER (either 1 or 4). */ static double parse_number (const char *nptr, int base, int radix, int radix_multiplier, char expchar, char **endptr) { const char *s = nptr; bool got_dot = false; long int exponent = 0; double num = 0; for (;; ++s) { int digit; if (c_isdigit (*s)) digit = *s - '0'; else if (base == 16 && c_isxdigit (*s)) digit = c_tolower (*s) - ('a' - 10); else if (! got_dot && *s == '.') { /* Record that we have found the decimal point. */ got_dot = true; continue; } else /* Any other character terminates the number. */ break; /* Make sure that multiplication by base will not overflow. */ if (num <= DBL_MAX / base) num = num * base + digit; else { /* The value of the digit doesn't matter, since we have already gotten as many digits as can be represented in a 'double'. This doesn't necessarily mean the result will overflow. The exponent may reduce it to within range. We just need to record that there was another digit so that we can multiply by 10 later. */ exponent += radix_multiplier; } /* Keep track of the number of digits after the decimal point. If we just divided by base here, we might lose precision. */ if (got_dot) exponent -= radix_multiplier; } if (c_tolower (*s) == expchar && ! locale_isspace (s[1])) { /* Add any given exponent to the implicit one. */ int save = errno; char *end; long int value = strtol (s + 1, &end, 10); errno = save; if (s + 1 != end) { /* Skip past the exponent, and add in the implicit exponent, resulting in an extreme value on overflow. */ s = end; exponent = (exponent < 0 ? (value < LONG_MIN - exponent ? LONG_MIN : exponent + value) : (LONG_MAX - exponent < value ? LONG_MAX : exponent + value)); } } *endptr = (char *) s; return scale_radix_exp (num, radix, exponent); } static double underlying_strtod (const char *, char **); /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0. ICC 10.0 has a bug when optimizing the expression -zero. The expression -DBL_MIN * DBL_MIN does not work when cross-compiling to PowerPC on Mac OS X 10.5. */ #if defined __hpux || defined __sgi || defined __ICC static double compute_minus_zero (void) { return -DBL_MIN * DBL_MIN; } # define minus_zero compute_minus_zero () #else double minus_zero = -0.0; #endif /* Convert NPTR to a double. If ENDPTR is not NULL, a pointer to the character after the last one used in the number is put in *ENDPTR. */ double strtod (const char *nptr, char **endptr) { bool negative = false; /* The number so far. */ double num; const char *s = nptr; const char *end; char *endbuf; int saved_errno = errno; /* Eat whitespace. */ while (locale_isspace (*s)) ++s; /* Get the sign. */ negative = *s == '-'; if (*s == '-' || *s == '+') ++s; num = underlying_strtod (s, &endbuf); end = endbuf; if (c_isdigit (s[*s == '.'])) { /* If a hex float was converted incorrectly, do it ourselves. If the string starts with "0x" but does not contain digits, consume the "0" ourselves. If a hex float is followed by a 'p' but no exponent, then adjust the end pointer. */ if (*s == '0' && c_tolower (s[1]) == 'x') { if (! c_isxdigit (s[2 + (s[2] == '.')])) { end = s + 1; /* strtod() on z/OS returns ERANGE for "0x". */ errno = saved_errno; } else if (end <= s + 2) { num = parse_number (s + 2, 16, 2, 4, 'p', &endbuf); end = endbuf; } else { const char *p = s + 2; while (p < end && c_tolower (*p) != 'p') p++; if (p < end && ! c_isdigit (p[1 + (p[1] == '-' || p[1] == '+')])) end = p; } } else { /* If "1e 1" was misparsed as 10.0 instead of 1.0, re-do the underlying strtod on a copy of the original string truncated to avoid the bug. */ const char *e = s + 1; while (e < end && c_tolower (*e) != 'e') e++; if (e < end && ! c_isdigit (e[1 + (e[1] == '-' || e[1] == '+')])) { char *dup = strdup (s); errno = saved_errno; if (!dup) { /* Not really our day, is it. Rounding errors are better than outright failure. */ num = parse_number (s, 10, 10, 1, 'e', &endbuf); } else { dup[e - s] = '\0'; num = underlying_strtod (dup, &endbuf); saved_errno = errno; free (dup); errno = saved_errno; } end = e; } } s = end; } /* Check for infinities and NaNs. */ else if (c_tolower (*s) == 'i' && c_tolower (s[1]) == 'n' && c_tolower (s[2]) == 'f') { s += 3; if (c_tolower (*s) == 'i' && c_tolower (s[1]) == 'n' && c_tolower (s[2]) == 'i' && c_tolower (s[3]) == 't' && c_tolower (s[4]) == 'y') s += 5; num = HUGE_VAL; errno = saved_errno; } else if (c_tolower (*s) == 'n' && c_tolower (s[1]) == 'a' && c_tolower (s[2]) == 'n') { s += 3; if (*s == '(') { const char *p = s + 1; while (c_isalnum (*p)) p++; if (*p == ')') s = p + 1; } /* If the underlying implementation misparsed the NaN, assume its result is incorrect, and return a NaN. Normally it's better to use the underlying implementation's result, since a nice implementation populates the bits of the NaN according to interpreting n-char-sequence as a hexadecimal number. */ if (s != end || num == num) num = NAN; errno = saved_errno; } else { /* No conversion could be performed. */ errno = EINVAL; s = nptr; } if (endptr != NULL) *endptr = (char *) s; /* Special case -0.0, since at least ICC miscompiles negation. We can't use copysign(), as that drags in -lm on some platforms. */ if (!num && negative) return minus_zero; return negative ? -num : num; } /* The underlying strtod implementation. This must be defined after strtod because it #undefs strtod. */ static double underlying_strtod (const char *nptr, char **endptr) { #undef strtod return strtod (nptr, endptr); } gnuastro-0.5/bootstrapped/lib/strnlen.c0000644000175000017500000000216513217200021015236 00000000000000/* Find the length of STRING, but scan at most MAXLEN characters. Copyright (C) 2005-2007, 2009-2017 Free Software Foundation, Inc. Written by Simon Josefsson. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include /* Find the length of STRING, but scan at most MAXLEN characters. If no '\0' terminator is found in that many characters, return MAXLEN. */ size_t strnlen (const char *string, size_t maxlen) { const char *end = memchr (string, '\0', maxlen); return end ? (size_t) (end - string) : maxlen; } gnuastro-0.5/bootstrapped/lib/strndup.c0000644000175000017500000000202513217200021015243 00000000000000/* A replacement function, for systems that lack strndup. Copyright (C) 1996-1998, 2001-2003, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include #include #include char * strndup (char const *s, size_t n) { size_t len = strnlen (s, n); char *new = malloc (len + 1); if (new == NULL) return NULL; new[len] = '\0'; return memcpy (new, s, len); } gnuastro-0.5/bootstrapped/lib/strerror-override.c0000644000175000017500000002146613217200021017255 00000000000000/* strerror-override.c --- POSIX compatible system error routine Copyright (C) 2010-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible , 2010. */ #include #include "strerror-override.h" #include #if GNULIB_defined_EWINSOCK /* native Windows platforms */ # if HAVE_WINSOCK2_H # include # endif #endif /* If ERRNUM maps to an errno value defined by gnulib, return a string describing the error. Otherwise return NULL. */ const char * strerror_override (int errnum) { /* These error messages are taken from glibc/sysdeps/gnu/errlist.c. */ switch (errnum) { #if REPLACE_STRERROR_0 case 0: return "Success"; #endif #if GNULIB_defined_ESOCK /* native Windows platforms with older */ case EINPROGRESS: return "Operation now in progress"; case EALREADY: return "Operation already in progress"; case ENOTSOCK: return "Socket operation on non-socket"; case EDESTADDRREQ: return "Destination address required"; case EMSGSIZE: return "Message too long"; case EPROTOTYPE: return "Protocol wrong type for socket"; case ENOPROTOOPT: return "Protocol not available"; case EPROTONOSUPPORT: return "Protocol not supported"; case EOPNOTSUPP: return "Operation not supported"; case EAFNOSUPPORT: return "Address family not supported by protocol"; case EADDRINUSE: return "Address already in use"; case EADDRNOTAVAIL: return "Cannot assign requested address"; case ENETDOWN: return "Network is down"; case ENETUNREACH: return "Network is unreachable"; case ECONNRESET: return "Connection reset by peer"; case ENOBUFS: return "No buffer space available"; case EISCONN: return "Transport endpoint is already connected"; case ENOTCONN: return "Transport endpoint is not connected"; case ETIMEDOUT: return "Connection timed out"; case ECONNREFUSED: return "Connection refused"; case ELOOP: return "Too many levels of symbolic links"; case EHOSTUNREACH: return "No route to host"; case EWOULDBLOCK: return "Operation would block"; #endif #if GNULIB_defined_ESTREAMS /* native Windows platforms with older */ case ETXTBSY: return "Text file busy"; case ENODATA: return "No data available"; case ENOSR: return "Out of streams resources"; case ENOSTR: return "Device not a stream"; case ETIME: return "Timer expired"; case EOTHER: return "Other error"; #endif #if GNULIB_defined_EWINSOCK /* native Windows platforms */ case ESOCKTNOSUPPORT: return "Socket type not supported"; case EPFNOSUPPORT: return "Protocol family not supported"; case ESHUTDOWN: return "Cannot send after transport endpoint shutdown"; case ETOOMANYREFS: return "Too many references: cannot splice"; case EHOSTDOWN: return "Host is down"; case EPROCLIM: return "Too many processes"; case EUSERS: return "Too many users"; case EDQUOT: return "Disk quota exceeded"; case ESTALE: return "Stale NFS file handle"; case EREMOTE: return "Object is remote"; # if HAVE_WINSOCK2_H /* WSA_INVALID_HANDLE maps to EBADF */ /* WSA_NOT_ENOUGH_MEMORY maps to ENOMEM */ /* WSA_INVALID_PARAMETER maps to EINVAL */ case WSA_OPERATION_ABORTED: return "Overlapped operation aborted"; case WSA_IO_INCOMPLETE: return "Overlapped I/O event object not in signaled state"; case WSA_IO_PENDING: return "Overlapped operations will complete later"; /* WSAEINTR maps to EINTR */ /* WSAEBADF maps to EBADF */ /* WSAEACCES maps to EACCES */ /* WSAEFAULT maps to EFAULT */ /* WSAEINVAL maps to EINVAL */ /* WSAEMFILE maps to EMFILE */ /* WSAEWOULDBLOCK maps to EWOULDBLOCK */ /* WSAEINPROGRESS maps to EINPROGRESS */ /* WSAEALREADY maps to EALREADY */ /* WSAENOTSOCK maps to ENOTSOCK */ /* WSAEDESTADDRREQ maps to EDESTADDRREQ */ /* WSAEMSGSIZE maps to EMSGSIZE */ /* WSAEPROTOTYPE maps to EPROTOTYPE */ /* WSAENOPROTOOPT maps to ENOPROTOOPT */ /* WSAEPROTONOSUPPORT maps to EPROTONOSUPPORT */ /* WSAESOCKTNOSUPPORT is ESOCKTNOSUPPORT */ /* WSAEOPNOTSUPP maps to EOPNOTSUPP */ /* WSAEPFNOSUPPORT is EPFNOSUPPORT */ /* WSAEAFNOSUPPORT maps to EAFNOSUPPORT */ /* WSAEADDRINUSE maps to EADDRINUSE */ /* WSAEADDRNOTAVAIL maps to EADDRNOTAVAIL */ /* WSAENETDOWN maps to ENETDOWN */ /* WSAENETUNREACH maps to ENETUNREACH */ /* WSAENETRESET maps to ENETRESET */ /* WSAECONNABORTED maps to ECONNABORTED */ /* WSAECONNRESET maps to ECONNRESET */ /* WSAENOBUFS maps to ENOBUFS */ /* WSAEISCONN maps to EISCONN */ /* WSAENOTCONN maps to ENOTCONN */ /* WSAESHUTDOWN is ESHUTDOWN */ /* WSAETOOMANYREFS is ETOOMANYREFS */ /* WSAETIMEDOUT maps to ETIMEDOUT */ /* WSAECONNREFUSED maps to ECONNREFUSED */ /* WSAELOOP maps to ELOOP */ /* WSAENAMETOOLONG maps to ENAMETOOLONG */ /* WSAEHOSTDOWN is EHOSTDOWN */ /* WSAEHOSTUNREACH maps to EHOSTUNREACH */ /* WSAENOTEMPTY maps to ENOTEMPTY */ /* WSAEPROCLIM is EPROCLIM */ /* WSAEUSERS is EUSERS */ /* WSAEDQUOT is EDQUOT */ /* WSAESTALE is ESTALE */ /* WSAEREMOTE is EREMOTE */ case WSASYSNOTREADY: return "Network subsystem is unavailable"; case WSAVERNOTSUPPORTED: return "Winsock.dll version out of range"; case WSANOTINITIALISED: return "Successful WSAStartup not yet performed"; case WSAEDISCON: return "Graceful shutdown in progress"; case WSAENOMORE: case WSA_E_NO_MORE: return "No more results"; case WSAECANCELLED: case WSA_E_CANCELLED: return "Call was canceled"; case WSAEINVALIDPROCTABLE: return "Procedure call table is invalid"; case WSAEINVALIDPROVIDER: return "Service provider is invalid"; case WSAEPROVIDERFAILEDINIT: return "Service provider failed to initialize"; case WSASYSCALLFAILURE: return "System call failure"; case WSASERVICE_NOT_FOUND: return "Service not found"; case WSATYPE_NOT_FOUND: return "Class type not found"; case WSAEREFUSED: return "Database query was refused"; case WSAHOST_NOT_FOUND: return "Host not found"; case WSATRY_AGAIN: return "Nonauthoritative host not found"; case WSANO_RECOVERY: return "Nonrecoverable error"; case WSANO_DATA: return "Valid name, no data record of requested type"; /* WSA_QOS_* omitted */ # endif #endif #if GNULIB_defined_ENOMSG case ENOMSG: return "No message of desired type"; #endif #if GNULIB_defined_EIDRM case EIDRM: return "Identifier removed"; #endif #if GNULIB_defined_ENOLINK case ENOLINK: return "Link has been severed"; #endif #if GNULIB_defined_EPROTO case EPROTO: return "Protocol error"; #endif #if GNULIB_defined_EMULTIHOP case EMULTIHOP: return "Multihop attempted"; #endif #if GNULIB_defined_EBADMSG case EBADMSG: return "Bad message"; #endif #if GNULIB_defined_EOVERFLOW case EOVERFLOW: return "Value too large for defined data type"; #endif #if GNULIB_defined_ENOTSUP case ENOTSUP: return "Not supported"; #endif #if GNULIB_defined_ENETRESET case ENETRESET: return "Network dropped connection on reset"; #endif #if GNULIB_defined_ECONNABORTED case ECONNABORTED: return "Software caused connection abort"; #endif #if GNULIB_defined_ESTALE case ESTALE: return "Stale NFS file handle"; #endif #if GNULIB_defined_EDQUOT case EDQUOT: return "Disk quota exceeded"; #endif #if GNULIB_defined_ECANCELED case ECANCELED: return "Operation canceled"; #endif #if GNULIB_defined_EOWNERDEAD case EOWNERDEAD: return "Owner died"; #endif #if GNULIB_defined_ENOTRECOVERABLE case ENOTRECOVERABLE: return "State not recoverable"; #endif #if GNULIB_defined_EILSEQ case EILSEQ: return "Invalid or incomplete multibyte or wide character"; #endif default: return NULL; } } gnuastro-0.5/bootstrapped/lib/strerror.c0000644000175000017500000000405313217200021015431 00000000000000/* strerror.c --- POSIX compatible system error routine Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #include #include #include "intprops.h" #include "strerror-override.h" #include "verify.h" /* Use the system functions, not the gnulib overrides in this file. */ #undef sprintf char * strerror (int n) #undef strerror { static char buf[STACKBUF_LEN]; size_t len; /* Cast away const, due to the historical signature of strerror; callers should not be modifying the string. */ const char *msg = strerror_override (n); if (msg) return (char *) msg; msg = strerror (n); /* Our strerror_r implementation might use the system's strerror buffer, so all other clients of strerror have to see the error copied into a buffer that we manage. This is not thread-safe, even if the system strerror is, but portable programs shouldn't be using strerror if they care about thread-safety. */ if (!msg || !*msg) { static char const fmt[] = "Unknown error %d"; verify (sizeof buf >= sizeof (fmt) + INT_STRLEN_BOUND (n)); sprintf (buf, fmt, n); errno = EINVAL; return buf; } /* Fix STACKBUF_LEN if this ever aborts. */ len = strlen (msg); if (sizeof buf <= len) abort (); memcpy (buf, msg, len + 1); return buf; } gnuastro-0.5/bootstrapped/lib/strchrnul.c0000644000175000017500000001301613217200021015572 00000000000000/* Searching in a string. Copyright (C) 2003, 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include /* Find the first occurrence of C in S or the final NUL byte. */ char * strchrnul (const char *s, int c_in) { /* On 32-bit hardware, choosing longword to be a 32-bit unsigned long instead of a 64-bit uintmax_t tends to give better performance. On 64-bit hardware, unsigned long is generally 64 bits already. Change this typedef to experiment with performance. */ typedef unsigned long int longword; const unsigned char *char_ptr; const longword *longword_ptr; longword repeated_one; longword repeated_c; unsigned char c; c = (unsigned char) c_in; if (!c) return rawmemchr (s, 0); /* Handle the first few bytes by reading one byte at a time. Do this until CHAR_PTR is aligned on a longword boundary. */ for (char_ptr = (const unsigned char *) s; (size_t) char_ptr % sizeof (longword) != 0; ++char_ptr) if (!*char_ptr || *char_ptr == c) return (char *) char_ptr; longword_ptr = (const longword *) char_ptr; /* All these elucidatory comments refer to 4-byte longwords, but the theory applies equally well to any size longwords. */ /* Compute auxiliary longword values: repeated_one is a value which has a 1 in every byte. repeated_c has c in every byte. */ repeated_one = 0x01010101; repeated_c = c | (c << 8); repeated_c |= repeated_c << 16; if (0xffffffffU < (longword) -1) { repeated_one |= repeated_one << 31 << 1; repeated_c |= repeated_c << 31 << 1; if (8 < sizeof (longword)) { size_t i; for (i = 64; i < sizeof (longword) * 8; i *= 2) { repeated_one |= repeated_one << i; repeated_c |= repeated_c << i; } } } /* Instead of the traditional loop which tests each byte, we will test a longword at a time. The tricky part is testing if *any of the four* bytes in the longword in question are equal to NUL or c. We first use an xor with repeated_c. This reduces the task to testing whether *any of the four* bytes in longword1 or longword2 is zero. Let's consider longword1. We compute tmp = ((longword1 - repeated_one) & ~longword1) & (repeated_one << 7). That is, we perform the following operations: 1. Subtract repeated_one. 2. & ~longword1. 3. & a mask consisting of 0x80 in every byte. Consider what happens in each byte: - If a byte of longword1 is zero, step 1 and 2 transform it into 0xff, and step 3 transforms it into 0x80. A carry can also be propagated to more significant bytes. - If a byte of longword1 is nonzero, let its lowest 1 bit be at position k (0 <= k <= 7); so the lowest k bits are 0. After step 1, the byte ends in a single bit of value 0 and k bits of value 1. After step 2, the result is just k bits of value 1: 2^k - 1. After step 3, the result is 0. And no carry is produced. So, if longword1 has only non-zero bytes, tmp is zero. Whereas if longword1 has a zero byte, call j the position of the least significant zero byte. Then the result has a zero at positions 0, ..., j-1 and a 0x80 at position j. We cannot predict the result at the more significant bytes (positions j+1..3), but it does not matter since we already have a non-zero bit at position 8*j+7. The test whether any byte in longword1 or longword2 is zero is equivalent to testing whether tmp1 is nonzero or tmp2 is nonzero. We can combine this into a single test, whether (tmp1 | tmp2) is nonzero. This test can read more than one byte beyond the end of a string, depending on where the terminating NUL is encountered. However, this is considered safe since the initialization phase ensured that the read will be aligned, therefore, the read will not cross page boundaries and will not cause a fault. */ while (1) { longword longword1 = *longword_ptr ^ repeated_c; longword longword2 = *longword_ptr; if (((((longword1 - repeated_one) & ~longword1) | ((longword2 - repeated_one) & ~longword2)) & (repeated_one << 7)) != 0) break; longword_ptr++; } char_ptr = (const unsigned char *) longword_ptr; /* At this point, we know that one of the sizeof (longword) bytes starting at char_ptr is == 0 or == c. On little-endian machines, we could determine the first such byte without any further memory accesses, just by looking at the tmp result from the last loop iteration. But this does not work on big-endian machines. Choose code that works in both cases. */ char_ptr = (unsigned char *) longword_ptr; while (*char_ptr && (*char_ptr != c)) char_ptr++; return (char *) char_ptr; } gnuastro-0.5/bootstrapped/lib/strncasecmp.c0000644000175000017500000000356013217200021016073 00000000000000/* strncasecmp.c -- case insensitive string comparator Copyright (C) 1998-1999, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include #include #include #define TOLOWER(Ch) (isupper (Ch) ? tolower (Ch) : (Ch)) /* Compare no more than N bytes of strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function cannot work correctly in multibyte locales. */ int strncasecmp (const char *s1, const char *s2, size_t n) { register const unsigned char *p1 = (const unsigned char *) s1; register const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2 || n == 0) return 0; do { c1 = TOLOWER (*p1); c2 = TOLOWER (*p2); if (--n == 0 || c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.5/bootstrapped/lib/strcasecmp.c0000644000175000017500000000343013217200021015711 00000000000000/* Case-insensitive string comparison function. Copyright (C) 1998-1999, 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include #include #include #define TOLOWER(Ch) (isupper (Ch) ? tolower (Ch) : (Ch)) /* Compare strings S1 and S2, ignoring case, returning less than, equal to or greater than zero if S1 is lexicographically less than, equal to or greater than S2. Note: This function does not work with multibyte strings! */ int strcasecmp (const char *s1, const char *s2) { const unsigned char *p1 = (const unsigned char *) s1; const unsigned char *p2 = (const unsigned char *) s2; unsigned char c1, c2; if (p1 == p2) return 0; do { c1 = TOLOWER (*p1); c2 = TOLOWER (*p2); if (c1 == '\0') break; ++p1; ++p2; } while (c1 == c2); if (UCHAR_MAX <= INT_MAX) return c1 - c2; else /* On machines where 'char' and 'int' are types of the same size, the difference of two 'unsigned char' values - including the sign bit - doesn't fit in an 'int'. */ return (c1 > c2 ? 1 : c1 < c2 ? -1 : 0); } gnuastro-0.5/bootstrapped/lib/sleep.c0000644000175000017500000000441013217200021014654 00000000000000/* Pausing execution of the current thread. Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include "verify.h" #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include unsigned int sleep (unsigned int seconds) { unsigned int remaining; /* Sleep for 1 second many times, because 1. Sleep is not interruptible by Ctrl-C, 2. we want to avoid arithmetic overflow while multiplying with 1000. */ for (remaining = seconds; remaining > 0; remaining--) Sleep (1000); return remaining; } #elif HAVE_SLEEP # undef sleep /* Guarantee unlimited sleep and a reasonable return value. Cygwin 1.5.x rejects attempts to sleep more than 49.7 days (2**32 milliseconds), but uses uninitialized memory which results in a garbage answer. Similarly, Linux 2.6.9 with glibc 2.3.4 has a too small return value when asked to sleep more than 24.85 days. */ unsigned int rpl_sleep (unsigned int seconds) { /* This requires int larger than 16 bits. */ verify (UINT_MAX / 24 / 24 / 60 / 60); const unsigned int limit = 24 * 24 * 60 * 60; while (limit < seconds) { unsigned int result; seconds -= limit; result = sleep (limit); if (result) return seconds + result; } return sleep (seconds); } #else /* !HAVE_SLEEP */ #error "Please port gnulib sleep.c to your platform, possibly using usleep() or select(), then report this to bug-gnulib." #endif gnuastro-0.5/bootstrapped/lib/regexec.c0000644000175000017500000037245213217200021015204 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ static reg_errcode_t match_ctx_init (re_match_context_t *cache, int eflags, Idx n); static void match_ctx_clean (re_match_context_t *mctx); static void match_ctx_free (re_match_context_t *cache); static reg_errcode_t match_ctx_add_entry (re_match_context_t *cache, Idx node, Idx str_idx, Idx from, Idx to); static Idx search_cur_bkref_entry (const re_match_context_t *mctx, Idx str_idx); static reg_errcode_t match_ctx_add_subtop (re_match_context_t *mctx, Idx node, Idx str_idx); static re_sub_match_last_t * match_ctx_add_sublast (re_sub_match_top_t *subtop, Idx node, Idx str_idx); static void sift_ctx_init (re_sift_context_t *sctx, re_dfastate_t **sifted_sts, re_dfastate_t **limited_sts, Idx last_node, Idx last_str_idx); static reg_errcode_t re_search_internal (const regex_t *preg, const char *string, Idx length, Idx start, Idx last_start, Idx stop, size_t nmatch, regmatch_t pmatch[], int eflags); static regoff_t re_search_2_stub (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, regoff_t range, struct re_registers *regs, Idx stop, bool ret_len); static regoff_t re_search_stub (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, regoff_t range, Idx stop, struct re_registers *regs, bool ret_len); static unsigned re_copy_regs (struct re_registers *regs, regmatch_t *pmatch, Idx nregs, int regs_allocated); static reg_errcode_t prune_impossible_nodes (re_match_context_t *mctx); static Idx check_matching (re_match_context_t *mctx, bool fl_longest_match, Idx *p_match_first); static Idx check_halt_state_context (const re_match_context_t *mctx, const re_dfastate_t *state, Idx idx); static void update_regs (const re_dfa_t *dfa, regmatch_t *pmatch, regmatch_t *prev_idx_match, Idx cur_node, Idx cur_idx, Idx nmatch); static reg_errcode_t push_fail_stack (struct re_fail_stack_t *fs, Idx str_idx, Idx dest_node, Idx nregs, regmatch_t *regs, re_node_set *eps_via_nodes); static reg_errcode_t set_regs (const regex_t *preg, const re_match_context_t *mctx, size_t nmatch, regmatch_t *pmatch, bool fl_backtrack); static reg_errcode_t free_fail_stack_return (struct re_fail_stack_t *fs); #ifdef RE_ENABLE_I18N static int sift_states_iter_mb (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx node_idx, Idx str_idx, Idx max_str_idx); #endif /* RE_ENABLE_I18N */ static reg_errcode_t sift_states_backward (const re_match_context_t *mctx, re_sift_context_t *sctx); static reg_errcode_t build_sifted_states (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *cur_dest); static reg_errcode_t update_cur_sifted_state (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *dest_nodes); static reg_errcode_t add_epsilon_src_nodes (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates); static bool check_dst_limits (const re_match_context_t *mctx, const re_node_set *limits, Idx dst_node, Idx dst_idx, Idx src_node, Idx src_idx); static int check_dst_limits_calc_pos_1 (const re_match_context_t *mctx, int boundaries, Idx subexp_idx, Idx from_node, Idx bkref_idx); static int check_dst_limits_calc_pos (const re_match_context_t *mctx, Idx limit, Idx subexp_idx, Idx node, Idx str_idx, Idx bkref_idx); static reg_errcode_t check_subexp_limits (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates, re_node_set *limits, struct re_backref_cache_entry *bkref_ents, Idx str_idx); static reg_errcode_t sift_states_bkref (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, const re_node_set *candidates); static reg_errcode_t merge_state_array (const re_dfa_t *dfa, re_dfastate_t **dst, re_dfastate_t **src, Idx num); static re_dfastate_t *find_recover_state (reg_errcode_t *err, re_match_context_t *mctx); static re_dfastate_t *transit_state (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *state); static re_dfastate_t *merge_state_with_log (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *next_state); static reg_errcode_t check_subexp_matching_top (re_match_context_t *mctx, re_node_set *cur_nodes, Idx str_idx); #if 0 static re_dfastate_t *transit_state_sb (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *pstate); #endif #ifdef RE_ENABLE_I18N static reg_errcode_t transit_state_mb (re_match_context_t *mctx, re_dfastate_t *pstate); #endif /* RE_ENABLE_I18N */ static reg_errcode_t transit_state_bkref (re_match_context_t *mctx, const re_node_set *nodes); static reg_errcode_t get_subexp (re_match_context_t *mctx, Idx bkref_node, Idx bkref_str_idx); static reg_errcode_t get_subexp_sub (re_match_context_t *mctx, const re_sub_match_top_t *sub_top, re_sub_match_last_t *sub_last, Idx bkref_node, Idx bkref_str); static Idx find_subexp_node (const re_dfa_t *dfa, const re_node_set *nodes, Idx subexp_idx, int type); static reg_errcode_t check_arrival (re_match_context_t *mctx, state_array_t *path, Idx top_node, Idx top_str, Idx last_node, Idx last_str, int type); static reg_errcode_t check_arrival_add_next_nodes (re_match_context_t *mctx, Idx str_idx, re_node_set *cur_nodes, re_node_set *next_nodes); static reg_errcode_t check_arrival_expand_ecl (const re_dfa_t *dfa, re_node_set *cur_nodes, Idx ex_subexp, int type); static reg_errcode_t check_arrival_expand_ecl_sub (const re_dfa_t *dfa, re_node_set *dst_nodes, Idx target, Idx ex_subexp, int type); static reg_errcode_t expand_bkref_cache (re_match_context_t *mctx, re_node_set *cur_nodes, Idx cur_str, Idx subexp_num, int type); static bool build_trtable (const re_dfa_t *dfa, re_dfastate_t *state); #ifdef RE_ENABLE_I18N static int check_node_accept_bytes (const re_dfa_t *dfa, Idx node_idx, const re_string_t *input, Idx idx); # ifdef _LIBC static unsigned int find_collation_sequence_value (const unsigned char *mbs, size_t name_len); # endif /* _LIBC */ #endif /* RE_ENABLE_I18N */ static Idx group_nodes_into_DFAstates (const re_dfa_t *dfa, const re_dfastate_t *state, re_node_set *states_node, bitset_t *states_ch); static bool check_node_accept (const re_match_context_t *mctx, const re_token_t *node, Idx idx); static reg_errcode_t extend_buffers (re_match_context_t *mctx, int min_len); /* Entry point for POSIX code. */ /* regexec searches for a given pattern, specified by PREG, in the string STRING. If NMATCH is zero or REG_NOSUB was set in the cflags argument to 'regcomp', we ignore PMATCH. Otherwise, we assume PMATCH has at least NMATCH elements, and we set them to the offsets of the corresponding matched substrings. EFLAGS specifies "execution flags" which affect matching: if REG_NOTBOL is set, then ^ does not match at the beginning of the string; if REG_NOTEOL is set, then $ does not match at the end. We return 0 if we find a match and REG_NOMATCH if not. */ int regexec (const regex_t *_Restrict_ preg, const char *_Restrict_ string, size_t nmatch, regmatch_t pmatch[], int eflags) { reg_errcode_t err; Idx start, length; re_dfa_t *dfa = preg->buffer; if (eflags & ~(REG_NOTBOL | REG_NOTEOL | REG_STARTEND)) return REG_BADPAT; if (eflags & REG_STARTEND) { start = pmatch[0].rm_so; length = pmatch[0].rm_eo; } else { start = 0; length = strlen (string); } lock_lock (dfa->lock); if (preg->no_sub) err = re_search_internal (preg, string, length, start, length, length, 0, NULL, eflags); else err = re_search_internal (preg, string, length, start, length, length, nmatch, pmatch, eflags); lock_unlock (dfa->lock); return err != REG_NOERROR; } #ifdef _LIBC libc_hidden_def (__regexec) # include versioned_symbol (libc, __regexec, regexec, GLIBC_2_3_4); # if SHLIB_COMPAT (libc, GLIBC_2_0, GLIBC_2_3_4) __typeof__ (__regexec) __compat_regexec; int attribute_compat_text_section __compat_regexec (const regex_t *_Restrict_ preg, const char *_Restrict_ string, size_t nmatch, regmatch_t pmatch[], int eflags) { return regexec (preg, string, nmatch, pmatch, eflags & (REG_NOTBOL | REG_NOTEOL)); } compat_symbol (libc, __compat_regexec, regexec, GLIBC_2_0); # endif #endif /* Entry points for GNU code. */ /* re_match, re_search, re_match_2, re_search_2 The former two functions operate on STRING with length LENGTH, while the later two operate on concatenation of STRING1 and STRING2 with lengths LENGTH1 and LENGTH2, respectively. re_match() matches the compiled pattern in BUFP against the string, starting at index START. re_search() first tries matching at index START, then it tries to match starting from index START + 1, and so on. The last start position tried is START + RANGE. (Thus RANGE = 0 forces re_search to operate the same way as re_match().) The parameter STOP of re_{match,search}_2 specifies that no match exceeding the first STOP characters of the concatenation of the strings should be concerned. If REGS is not NULL, and BUFP->no_sub is not set, the offsets of the match and all groups is stored in REGS. (For the "_2" variants, the offsets are computed relative to the concatenation, not relative to the individual strings.) On success, re_match* functions return the length of the match, re_search* return the position of the start of the match. Return value -1 means no match was found and -2 indicates an internal error. */ regoff_t re_match (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, struct re_registers *regs) { return re_search_stub (bufp, string, length, start, 0, length, regs, true); } #ifdef _LIBC weak_alias (__re_match, re_match) #endif regoff_t re_search (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, regoff_t range, struct re_registers *regs) { return re_search_stub (bufp, string, length, start, range, length, regs, false); } #ifdef _LIBC weak_alias (__re_search, re_search) #endif regoff_t re_match_2 (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, struct re_registers *regs, Idx stop) { return re_search_2_stub (bufp, string1, length1, string2, length2, start, 0, regs, stop, true); } #ifdef _LIBC weak_alias (__re_match_2, re_match_2) #endif regoff_t re_search_2 (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, regoff_t range, struct re_registers *regs, Idx stop) { return re_search_2_stub (bufp, string1, length1, string2, length2, start, range, regs, stop, false); } #ifdef _LIBC weak_alias (__re_search_2, re_search_2) #endif static regoff_t re_search_2_stub (struct re_pattern_buffer *bufp, const char *string1, Idx length1, const char *string2, Idx length2, Idx start, regoff_t range, struct re_registers *regs, Idx stop, bool ret_len) { const char *str; regoff_t rval; Idx len; char *s = NULL; if (BE ((length1 < 0 || length2 < 0 || stop < 0 || INT_ADD_WRAPV (length1, length2, &len)), 0)) return -2; /* Concatenate the strings. */ if (length2 > 0) if (length1 > 0) { s = re_malloc (char, len); if (BE (s == NULL, 0)) return -2; #ifdef _LIBC memcpy (__mempcpy (s, string1, length1), string2, length2); #else memcpy (s, string1, length1); memcpy (s + length1, string2, length2); #endif str = s; } else str = string2; else str = string1; rval = re_search_stub (bufp, str, len, start, range, stop, regs, ret_len); re_free (s); return rval; } /* The parameters have the same meaning as those of re_search. Additional parameters: If RET_LEN is true the length of the match is returned (re_match style); otherwise the position of the match is returned. */ static regoff_t re_search_stub (struct re_pattern_buffer *bufp, const char *string, Idx length, Idx start, regoff_t range, Idx stop, struct re_registers *regs, bool ret_len) { reg_errcode_t result; regmatch_t *pmatch; Idx nregs; regoff_t rval; int eflags = 0; re_dfa_t *dfa = bufp->buffer; Idx last_start = start + range; /* Check for out-of-range. */ if (BE (start < 0 || start > length, 0)) return -1; if (BE (length < last_start || (0 <= range && last_start < start), 0)) last_start = length; else if (BE (last_start < 0 || (range < 0 && start <= last_start), 0)) last_start = 0; lock_lock (dfa->lock); eflags |= (bufp->not_bol) ? REG_NOTBOL : 0; eflags |= (bufp->not_eol) ? REG_NOTEOL : 0; /* Compile fastmap if we haven't yet. */ if (start < last_start && bufp->fastmap != NULL && !bufp->fastmap_accurate) re_compile_fastmap (bufp); if (BE (bufp->no_sub, 0)) regs = NULL; /* We need at least 1 register. */ if (regs == NULL) nregs = 1; else if (BE (bufp->regs_allocated == REGS_FIXED && regs->num_regs <= bufp->re_nsub, 0)) { nregs = regs->num_regs; if (BE (nregs < 1, 0)) { /* Nothing can be copied to regs. */ regs = NULL; nregs = 1; } } else nregs = bufp->re_nsub + 1; pmatch = re_malloc (regmatch_t, nregs); if (BE (pmatch == NULL, 0)) { rval = -2; goto out; } result = re_search_internal (bufp, string, length, start, last_start, stop, nregs, pmatch, eflags); rval = 0; /* I hope we needn't fill their regs with -1's when no match was found. */ if (result != REG_NOERROR) rval = result == REG_NOMATCH ? -1 : -2; else if (regs != NULL) { /* If caller wants register contents data back, copy them. */ bufp->regs_allocated = re_copy_regs (regs, pmatch, nregs, bufp->regs_allocated); if (BE (bufp->regs_allocated == REGS_UNALLOCATED, 0)) rval = -2; } if (BE (rval == 0, 1)) { if (ret_len) { assert (pmatch[0].rm_so == start); rval = pmatch[0].rm_eo - start; } else rval = pmatch[0].rm_so; } re_free (pmatch); out: lock_unlock (dfa->lock); return rval; } static unsigned re_copy_regs (struct re_registers *regs, regmatch_t *pmatch, Idx nregs, int regs_allocated) { int rval = REGS_REALLOCATE; Idx i; Idx need_regs = nregs + 1; /* We need one extra element beyond 'num_regs' for the '-1' marker GNU code uses. */ /* Have the register data arrays been allocated? */ if (regs_allocated == REGS_UNALLOCATED) { /* No. So allocate them with malloc. */ regs->start = re_malloc (regoff_t, need_regs); if (BE (regs->start == NULL, 0)) return REGS_UNALLOCATED; regs->end = re_malloc (regoff_t, need_regs); if (BE (regs->end == NULL, 0)) { re_free (regs->start); return REGS_UNALLOCATED; } regs->num_regs = need_regs; } else if (regs_allocated == REGS_REALLOCATE) { /* Yes. If we need more elements than were already allocated, reallocate them. If we need fewer, just leave it alone. */ if (BE (need_regs > regs->num_regs, 0)) { regoff_t *new_start = re_realloc (regs->start, regoff_t, need_regs); regoff_t *new_end; if (BE (new_start == NULL, 0)) return REGS_UNALLOCATED; new_end = re_realloc (regs->end, regoff_t, need_regs); if (BE (new_end == NULL, 0)) { re_free (new_start); return REGS_UNALLOCATED; } regs->start = new_start; regs->end = new_end; regs->num_regs = need_regs; } } else { assert (regs_allocated == REGS_FIXED); /* This function may not be called with REGS_FIXED and nregs too big. */ assert (regs->num_regs >= nregs); rval = REGS_FIXED; } /* Copy the regs. */ for (i = 0; i < nregs; ++i) { regs->start[i] = pmatch[i].rm_so; regs->end[i] = pmatch[i].rm_eo; } for ( ; i < regs->num_regs; ++i) regs->start[i] = regs->end[i] = -1; return rval; } /* Set REGS to hold NUM_REGS registers, storing them in STARTS and ENDS. Subsequent matches using PATTERN_BUFFER and REGS will use this memory for recording register information. STARTS and ENDS must be allocated using the malloc library routine, and must each be at least NUM_REGS * sizeof (regoff_t) bytes long. If NUM_REGS == 0, then subsequent matches should allocate their own register data. Unless this function is called, the first search or match using PATTERN_BUFFER will allocate its own register data, without freeing the old data. */ void re_set_registers (struct re_pattern_buffer *bufp, struct re_registers *regs, __re_size_t num_regs, regoff_t *starts, regoff_t *ends) { if (num_regs) { bufp->regs_allocated = REGS_REALLOCATE; regs->num_regs = num_regs; regs->start = starts; regs->end = ends; } else { bufp->regs_allocated = REGS_UNALLOCATED; regs->num_regs = 0; regs->start = regs->end = NULL; } } #ifdef _LIBC weak_alias (__re_set_registers, re_set_registers) #endif /* Entry points compatible with 4.2 BSD regex library. We don't define them unless specifically requested. */ #if defined _REGEX_RE_COMP || defined _LIBC int # ifdef _LIBC weak_function # endif re_exec (const char *s) { return 0 == regexec (&re_comp_buf, s, 0, NULL, 0); } #endif /* _REGEX_RE_COMP */ /* Internal entry point. */ /* Searches for a compiled pattern PREG in the string STRING, whose length is LENGTH. NMATCH, PMATCH, and EFLAGS have the same meaning as with regexec. LAST_START is START + RANGE, where START and RANGE have the same meaning as with re_search. Return REG_NOERROR if we find a match, and REG_NOMATCH if not, otherwise return the error code. Note: We assume front end functions already check ranges. (0 <= LAST_START && LAST_START <= LENGTH) */ static reg_errcode_t __attribute_warn_unused_result__ re_search_internal (const regex_t *preg, const char *string, Idx length, Idx start, Idx last_start, Idx stop, size_t nmatch, regmatch_t pmatch[], int eflags) { reg_errcode_t err; const re_dfa_t *dfa = preg->buffer; Idx left_lim, right_lim; int incr; bool fl_longest_match; int match_kind; Idx match_first; Idx match_last = -1; Idx extra_nmatch; bool sb; int ch; #if defined _LIBC || (defined __STDC_VERSION__ && __STDC_VERSION__ >= 199901L) re_match_context_t mctx = { .dfa = dfa }; #else re_match_context_t mctx; #endif char *fastmap = ((preg->fastmap != NULL && preg->fastmap_accurate && start != last_start && !preg->can_be_null) ? preg->fastmap : NULL); RE_TRANSLATE_TYPE t = preg->translate; #if !(defined _LIBC || (defined __STDC_VERSION__ && __STDC_VERSION__ >= 199901L)) memset (&mctx, '\0', sizeof (re_match_context_t)); mctx.dfa = dfa; #endif extra_nmatch = (nmatch > preg->re_nsub) ? nmatch - (preg->re_nsub + 1) : 0; nmatch -= extra_nmatch; /* Check if the DFA haven't been compiled. */ if (BE (preg->used == 0 || dfa->init_state == NULL || dfa->init_state_word == NULL || dfa->init_state_nl == NULL || dfa->init_state_begbuf == NULL, 0)) return REG_NOMATCH; #ifdef DEBUG /* We assume front-end functions already check them. */ assert (0 <= last_start && last_start <= length); #endif /* If initial states with non-begbuf contexts have no elements, the regex must be anchored. If preg->newline_anchor is set, we'll never use init_state_nl, so do not check it. */ if (dfa->init_state->nodes.nelem == 0 && dfa->init_state_word->nodes.nelem == 0 && (dfa->init_state_nl->nodes.nelem == 0 || !preg->newline_anchor)) { if (start != 0 && last_start != 0) return REG_NOMATCH; start = last_start = 0; } /* We must check the longest matching, if nmatch > 0. */ fl_longest_match = (nmatch != 0 || dfa->nbackref); err = re_string_allocate (&mctx.input, string, length, dfa->nodes_len + 1, preg->translate, (preg->syntax & RE_ICASE) != 0, dfa); if (BE (err != REG_NOERROR, 0)) goto free_return; mctx.input.stop = stop; mctx.input.raw_stop = stop; mctx.input.newline_anchor = preg->newline_anchor; err = match_ctx_init (&mctx, eflags, dfa->nbackref * 2); if (BE (err != REG_NOERROR, 0)) goto free_return; /* We will log all the DFA states through which the dfa pass, if nmatch > 1, or this dfa has "multibyte node", which is a back-reference or a node which can accept multibyte character or multi character collating element. */ if (nmatch > 1 || dfa->has_mb_node) { /* Avoid overflow. */ if (BE ((MIN (IDX_MAX, SIZE_MAX / sizeof (re_dfastate_t *)) <= mctx.input.bufs_len), 0)) { err = REG_ESPACE; goto free_return; } mctx.state_log = re_malloc (re_dfastate_t *, mctx.input.bufs_len + 1); if (BE (mctx.state_log == NULL, 0)) { err = REG_ESPACE; goto free_return; } } else mctx.state_log = NULL; match_first = start; mctx.input.tip_context = (eflags & REG_NOTBOL) ? CONTEXT_BEGBUF : CONTEXT_NEWLINE | CONTEXT_BEGBUF; /* Check incrementally whether the input string matches. */ incr = (last_start < start) ? -1 : 1; left_lim = (last_start < start) ? last_start : start; right_lim = (last_start < start) ? start : last_start; sb = dfa->mb_cur_max == 1; match_kind = (fastmap ? ((sb || !(preg->syntax & RE_ICASE || t) ? 4 : 0) | (start <= last_start ? 2 : 0) | (t != NULL ? 1 : 0)) : 8); for (;; match_first += incr) { err = REG_NOMATCH; if (match_first < left_lim || right_lim < match_first) goto free_return; /* Advance as rapidly as possible through the string, until we find a plausible place to start matching. This may be done with varying efficiency, so there are various possibilities: only the most common of them are specialized, in order to save on code size. We use a switch statement for speed. */ switch (match_kind) { case 8: /* No fastmap. */ break; case 7: /* Fastmap with single-byte translation, match forward. */ while (BE (match_first < right_lim, 1) && !fastmap[t[(unsigned char) string[match_first]]]) ++match_first; goto forward_match_found_start_or_reached_end; case 6: /* Fastmap without translation, match forward. */ while (BE (match_first < right_lim, 1) && !fastmap[(unsigned char) string[match_first]]) ++match_first; forward_match_found_start_or_reached_end: if (BE (match_first == right_lim, 0)) { ch = match_first >= length ? 0 : (unsigned char) string[match_first]; if (!fastmap[t ? t[ch] : ch]) goto free_return; } break; case 4: case 5: /* Fastmap without multi-byte translation, match backwards. */ while (match_first >= left_lim) { ch = match_first >= length ? 0 : (unsigned char) string[match_first]; if (fastmap[t ? t[ch] : ch]) break; --match_first; } if (match_first < left_lim) goto free_return; break; default: /* In this case, we can't determine easily the current byte, since it might be a component byte of a multibyte character. Then we use the constructed buffer instead. */ for (;;) { /* If MATCH_FIRST is out of the valid range, reconstruct the buffers. */ __re_size_t offset = match_first - mctx.input.raw_mbs_idx; if (BE (offset >= (__re_size_t) mctx.input.valid_raw_len, 0)) { err = re_string_reconstruct (&mctx.input, match_first, eflags); if (BE (err != REG_NOERROR, 0)) goto free_return; offset = match_first - mctx.input.raw_mbs_idx; } /* If MATCH_FIRST is out of the buffer, leave it as '\0'. Note that MATCH_FIRST must not be smaller than 0. */ ch = (match_first >= length ? 0 : re_string_byte_at (&mctx.input, offset)); if (fastmap[ch]) break; match_first += incr; if (match_first < left_lim || match_first > right_lim) { err = REG_NOMATCH; goto free_return; } } break; } /* Reconstruct the buffers so that the matcher can assume that the matching starts from the beginning of the buffer. */ err = re_string_reconstruct (&mctx.input, match_first, eflags); if (BE (err != REG_NOERROR, 0)) goto free_return; #ifdef RE_ENABLE_I18N /* Don't consider this char as a possible match start if it part, yet isn't the head, of a multibyte character. */ if (!sb && !re_string_first_byte (&mctx.input, 0)) continue; #endif /* It seems to be appropriate one, then use the matcher. */ /* We assume that the matching starts from 0. */ mctx.state_log_top = mctx.nbkref_ents = mctx.max_mb_elem_len = 0; match_last = check_matching (&mctx, fl_longest_match, start <= last_start ? &match_first : NULL); if (match_last != -1) { if (BE (match_last == -2, 0)) { err = REG_ESPACE; goto free_return; } else { mctx.match_last = match_last; if ((!preg->no_sub && nmatch > 1) || dfa->nbackref) { re_dfastate_t *pstate = mctx.state_log[match_last]; mctx.last_node = check_halt_state_context (&mctx, pstate, match_last); } if ((!preg->no_sub && nmatch > 1 && dfa->has_plural_match) || dfa->nbackref) { err = prune_impossible_nodes (&mctx); if (err == REG_NOERROR) break; if (BE (err != REG_NOMATCH, 0)) goto free_return; match_last = -1; } else break; /* We found a match. */ } } match_ctx_clean (&mctx); } #ifdef DEBUG assert (match_last != -1); assert (err == REG_NOERROR); #endif /* Set pmatch[] if we need. */ if (nmatch > 0) { Idx reg_idx; /* Initialize registers. */ for (reg_idx = 1; reg_idx < nmatch; ++reg_idx) pmatch[reg_idx].rm_so = pmatch[reg_idx].rm_eo = -1; /* Set the points where matching start/end. */ pmatch[0].rm_so = 0; pmatch[0].rm_eo = mctx.match_last; /* FIXME: This function should fail if mctx.match_last exceeds the maximum possible regoff_t value. We need a new error code REG_OVERFLOW. */ if (!preg->no_sub && nmatch > 1) { err = set_regs (preg, &mctx, nmatch, pmatch, dfa->has_plural_match && dfa->nbackref > 0); if (BE (err != REG_NOERROR, 0)) goto free_return; } /* At last, add the offset to each register, since we slid the buffers so that we could assume that the matching starts from 0. */ for (reg_idx = 0; reg_idx < nmatch; ++reg_idx) if (pmatch[reg_idx].rm_so != -1) { #ifdef RE_ENABLE_I18N if (BE (mctx.input.offsets_needed != 0, 0)) { pmatch[reg_idx].rm_so = (pmatch[reg_idx].rm_so == mctx.input.valid_len ? mctx.input.valid_raw_len : mctx.input.offsets[pmatch[reg_idx].rm_so]); pmatch[reg_idx].rm_eo = (pmatch[reg_idx].rm_eo == mctx.input.valid_len ? mctx.input.valid_raw_len : mctx.input.offsets[pmatch[reg_idx].rm_eo]); } #else assert (mctx.input.offsets_needed == 0); #endif pmatch[reg_idx].rm_so += match_first; pmatch[reg_idx].rm_eo += match_first; } for (reg_idx = 0; reg_idx < extra_nmatch; ++reg_idx) { pmatch[nmatch + reg_idx].rm_so = -1; pmatch[nmatch + reg_idx].rm_eo = -1; } if (dfa->subexp_map) for (reg_idx = 0; reg_idx + 1 < nmatch; reg_idx++) if (dfa->subexp_map[reg_idx] != reg_idx) { pmatch[reg_idx + 1].rm_so = pmatch[dfa->subexp_map[reg_idx] + 1].rm_so; pmatch[reg_idx + 1].rm_eo = pmatch[dfa->subexp_map[reg_idx] + 1].rm_eo; } } free_return: re_free (mctx.state_log); if (dfa->nbackref) match_ctx_free (&mctx); re_string_destruct (&mctx.input); return err; } static reg_errcode_t __attribute_warn_unused_result__ prune_impossible_nodes (re_match_context_t *mctx) { const re_dfa_t *const dfa = mctx->dfa; Idx halt_node, match_last; reg_errcode_t ret; re_dfastate_t **sifted_states; re_dfastate_t **lim_states = NULL; re_sift_context_t sctx; #ifdef DEBUG assert (mctx->state_log != NULL); #endif match_last = mctx->match_last; halt_node = mctx->last_node; /* Avoid overflow. */ if (BE (MIN (IDX_MAX, SIZE_MAX / sizeof (re_dfastate_t *)) <= match_last, 0)) return REG_ESPACE; sifted_states = re_malloc (re_dfastate_t *, match_last + 1); if (BE (sifted_states == NULL, 0)) { ret = REG_ESPACE; goto free_return; } if (dfa->nbackref) { lim_states = re_malloc (re_dfastate_t *, match_last + 1); if (BE (lim_states == NULL, 0)) { ret = REG_ESPACE; goto free_return; } while (1) { memset (lim_states, '\0', sizeof (re_dfastate_t *) * (match_last + 1)); sift_ctx_init (&sctx, sifted_states, lim_states, halt_node, match_last); ret = sift_states_backward (mctx, &sctx); re_node_set_free (&sctx.limits); if (BE (ret != REG_NOERROR, 0)) goto free_return; if (sifted_states[0] != NULL || lim_states[0] != NULL) break; do { --match_last; if (match_last < 0) { ret = REG_NOMATCH; goto free_return; } } while (mctx->state_log[match_last] == NULL || !mctx->state_log[match_last]->halt); halt_node = check_halt_state_context (mctx, mctx->state_log[match_last], match_last); } ret = merge_state_array (dfa, sifted_states, lim_states, match_last + 1); re_free (lim_states); lim_states = NULL; if (BE (ret != REG_NOERROR, 0)) goto free_return; } else { sift_ctx_init (&sctx, sifted_states, lim_states, halt_node, match_last); ret = sift_states_backward (mctx, &sctx); re_node_set_free (&sctx.limits); if (BE (ret != REG_NOERROR, 0)) goto free_return; if (sifted_states[0] == NULL) { ret = REG_NOMATCH; goto free_return; } } re_free (mctx->state_log); mctx->state_log = sifted_states; sifted_states = NULL; mctx->last_node = halt_node; mctx->match_last = match_last; ret = REG_NOERROR; free_return: re_free (sifted_states); re_free (lim_states); return ret; } /* Acquire an initial state and return it. We must select appropriate initial state depending on the context, since initial states may have constraints like "\<", "^", etc.. */ static inline re_dfastate_t * __attribute__ ((always_inline)) acquire_init_state_context (reg_errcode_t *err, const re_match_context_t *mctx, Idx idx) { const re_dfa_t *const dfa = mctx->dfa; if (dfa->init_state->has_constraint) { unsigned int context; context = re_string_context_at (&mctx->input, idx - 1, mctx->eflags); if (IS_WORD_CONTEXT (context)) return dfa->init_state_word; else if (IS_ORDINARY_CONTEXT (context)) return dfa->init_state; else if (IS_BEGBUF_CONTEXT (context) && IS_NEWLINE_CONTEXT (context)) return dfa->init_state_begbuf; else if (IS_NEWLINE_CONTEXT (context)) return dfa->init_state_nl; else if (IS_BEGBUF_CONTEXT (context)) { /* It is relatively rare case, then calculate on demand. */ return re_acquire_state_context (err, dfa, dfa->init_state->entrance_nodes, context); } else /* Must not happen? */ return dfa->init_state; } else return dfa->init_state; } /* Check whether the regular expression match input string INPUT or not, and return the index where the matching end. Return -1 if there is no match, and return -2 in case of an error. FL_LONGEST_MATCH means we want the POSIX longest matching. If P_MATCH_FIRST is not NULL, and the match fails, it is set to the next place where we may want to try matching. Note that the matcher assumes that the matching starts from the current index of the buffer. */ static Idx __attribute_warn_unused_result__ check_matching (re_match_context_t *mctx, bool fl_longest_match, Idx *p_match_first) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx match = 0; Idx match_last = -1; Idx cur_str_idx = re_string_cur_idx (&mctx->input); re_dfastate_t *cur_state; bool at_init_state = p_match_first != NULL; Idx next_start_idx = cur_str_idx; err = REG_NOERROR; cur_state = acquire_init_state_context (&err, mctx, cur_str_idx); /* An initial state must not be NULL (invalid). */ if (BE (cur_state == NULL, 0)) { assert (err == REG_ESPACE); return -2; } if (mctx->state_log != NULL) { mctx->state_log[cur_str_idx] = cur_state; /* Check OP_OPEN_SUBEXP in the initial state in case that we use them later. E.g. Processing back references. */ if (BE (dfa->nbackref, 0)) { at_init_state = false; err = check_subexp_matching_top (mctx, &cur_state->nodes, 0); if (BE (err != REG_NOERROR, 0)) return err; if (cur_state->has_backref) { err = transit_state_bkref (mctx, &cur_state->nodes); if (BE (err != REG_NOERROR, 0)) return err; } } } /* If the RE accepts NULL string. */ if (BE (cur_state->halt, 0)) { if (!cur_state->has_constraint || check_halt_state_context (mctx, cur_state, cur_str_idx)) { if (!fl_longest_match) return cur_str_idx; else { match_last = cur_str_idx; match = 1; } } } while (!re_string_eoi (&mctx->input)) { re_dfastate_t *old_state = cur_state; Idx next_char_idx = re_string_cur_idx (&mctx->input) + 1; if ((BE (next_char_idx >= mctx->input.bufs_len, 0) && mctx->input.bufs_len < mctx->input.len) || (BE (next_char_idx >= mctx->input.valid_len, 0) && mctx->input.valid_len < mctx->input.len)) { err = extend_buffers (mctx, next_char_idx + 1); if (BE (err != REG_NOERROR, 0)) { assert (err == REG_ESPACE); return -2; } } cur_state = transit_state (&err, mctx, cur_state); if (mctx->state_log != NULL) cur_state = merge_state_with_log (&err, mctx, cur_state); if (cur_state == NULL) { /* Reached the invalid state or an error. Try to recover a valid state using the state log, if available and if we have not already found a valid (even if not the longest) match. */ if (BE (err != REG_NOERROR, 0)) return -2; if (mctx->state_log == NULL || (match && !fl_longest_match) || (cur_state = find_recover_state (&err, mctx)) == NULL) break; } if (BE (at_init_state, 0)) { if (old_state == cur_state) next_start_idx = next_char_idx; else at_init_state = false; } if (cur_state->halt) { /* Reached a halt state. Check the halt state can satisfy the current context. */ if (!cur_state->has_constraint || check_halt_state_context (mctx, cur_state, re_string_cur_idx (&mctx->input))) { /* We found an appropriate halt state. */ match_last = re_string_cur_idx (&mctx->input); match = 1; /* We found a match, do not modify match_first below. */ p_match_first = NULL; if (!fl_longest_match) break; } } } if (p_match_first) *p_match_first += next_start_idx; return match_last; } /* Check NODE match the current context. */ static bool check_halt_node_context (const re_dfa_t *dfa, Idx node, unsigned int context) { re_token_type_t type = dfa->nodes[node].type; unsigned int constraint = dfa->nodes[node].constraint; if (type != END_OF_RE) return false; if (!constraint) return true; if (NOT_SATISFY_NEXT_CONSTRAINT (constraint, context)) return false; return true; } /* Check the halt state STATE match the current context. Return 0 if not match, if the node, STATE has, is a halt node and match the context, return the node. */ static Idx check_halt_state_context (const re_match_context_t *mctx, const re_dfastate_t *state, Idx idx) { Idx i; unsigned int context; #ifdef DEBUG assert (state->halt); #endif context = re_string_context_at (&mctx->input, idx, mctx->eflags); for (i = 0; i < state->nodes.nelem; ++i) if (check_halt_node_context (mctx->dfa, state->nodes.elems[i], context)) return state->nodes.elems[i]; return 0; } /* Compute the next node to which "NFA" transit from NODE("NFA" is a NFA corresponding to the DFA). Return the destination node, and update EPS_VIA_NODES; return -1 in case of errors. */ static Idx proceed_next_node (const re_match_context_t *mctx, Idx nregs, regmatch_t *regs, Idx *pidx, Idx node, re_node_set *eps_via_nodes, struct re_fail_stack_t *fs) { const re_dfa_t *const dfa = mctx->dfa; Idx i; bool ok; if (IS_EPSILON_NODE (dfa->nodes[node].type)) { re_node_set *cur_nodes = &mctx->state_log[*pidx]->nodes; re_node_set *edests = &dfa->edests[node]; Idx dest_node; ok = re_node_set_insert (eps_via_nodes, node); if (BE (! ok, 0)) return -2; /* Pick up a valid destination, or return -1 if none is found. */ for (dest_node = -1, i = 0; i < edests->nelem; ++i) { Idx candidate = edests->elems[i]; if (!re_node_set_contains (cur_nodes, candidate)) continue; if (dest_node == -1) dest_node = candidate; else { /* In order to avoid infinite loop like "(a*)*", return the second epsilon-transition if the first was already considered. */ if (re_node_set_contains (eps_via_nodes, dest_node)) return candidate; /* Otherwise, push the second epsilon-transition on the fail stack. */ else if (fs != NULL && push_fail_stack (fs, *pidx, candidate, nregs, regs, eps_via_nodes)) return -2; /* We know we are going to exit. */ break; } } return dest_node; } else { Idx naccepted = 0; re_token_type_t type = dfa->nodes[node].type; #ifdef RE_ENABLE_I18N if (dfa->nodes[node].accept_mb) naccepted = check_node_accept_bytes (dfa, node, &mctx->input, *pidx); else #endif /* RE_ENABLE_I18N */ if (type == OP_BACK_REF) { Idx subexp_idx = dfa->nodes[node].opr.idx + 1; naccepted = regs[subexp_idx].rm_eo - regs[subexp_idx].rm_so; if (fs != NULL) { if (regs[subexp_idx].rm_so == -1 || regs[subexp_idx].rm_eo == -1) return -1; else if (naccepted) { char *buf = (char *) re_string_get_buffer (&mctx->input); if (memcmp (buf + regs[subexp_idx].rm_so, buf + *pidx, naccepted) != 0) return -1; } } if (naccepted == 0) { Idx dest_node; ok = re_node_set_insert (eps_via_nodes, node); if (BE (! ok, 0)) return -2; dest_node = dfa->edests[node].elems[0]; if (re_node_set_contains (&mctx->state_log[*pidx]->nodes, dest_node)) return dest_node; } } if (naccepted != 0 || check_node_accept (mctx, dfa->nodes + node, *pidx)) { Idx dest_node = dfa->nexts[node]; *pidx = (naccepted == 0) ? *pidx + 1 : *pidx + naccepted; if (fs && (*pidx > mctx->match_last || mctx->state_log[*pidx] == NULL || !re_node_set_contains (&mctx->state_log[*pidx]->nodes, dest_node))) return -1; re_node_set_empty (eps_via_nodes); return dest_node; } } return -1; } static reg_errcode_t __attribute_warn_unused_result__ push_fail_stack (struct re_fail_stack_t *fs, Idx str_idx, Idx dest_node, Idx nregs, regmatch_t *regs, re_node_set *eps_via_nodes) { reg_errcode_t err; Idx num = fs->num++; if (fs->num == fs->alloc) { struct re_fail_stack_ent_t *new_array; new_array = re_realloc (fs->stack, struct re_fail_stack_ent_t, fs->alloc * 2); if (new_array == NULL) return REG_ESPACE; fs->alloc *= 2; fs->stack = new_array; } fs->stack[num].idx = str_idx; fs->stack[num].node = dest_node; fs->stack[num].regs = re_malloc (regmatch_t, nregs); if (fs->stack[num].regs == NULL) return REG_ESPACE; memcpy (fs->stack[num].regs, regs, sizeof (regmatch_t) * nregs); err = re_node_set_init_copy (&fs->stack[num].eps_via_nodes, eps_via_nodes); return err; } static Idx pop_fail_stack (struct re_fail_stack_t *fs, Idx *pidx, Idx nregs, regmatch_t *regs, re_node_set *eps_via_nodes) { Idx num = --fs->num; assert (num >= 0); *pidx = fs->stack[num].idx; memcpy (regs, fs->stack[num].regs, sizeof (regmatch_t) * nregs); re_node_set_free (eps_via_nodes); re_free (fs->stack[num].regs); *eps_via_nodes = fs->stack[num].eps_via_nodes; return fs->stack[num].node; } /* Set the positions where the subexpressions are starts/ends to registers PMATCH. Note: We assume that pmatch[0] is already set, and pmatch[i].rm_so == pmatch[i].rm_eo == -1 for 0 < i < nmatch. */ static reg_errcode_t __attribute_warn_unused_result__ set_regs (const regex_t *preg, const re_match_context_t *mctx, size_t nmatch, regmatch_t *pmatch, bool fl_backtrack) { const re_dfa_t *dfa = preg->buffer; Idx idx, cur_node; re_node_set eps_via_nodes; struct re_fail_stack_t *fs; struct re_fail_stack_t fs_body = { 0, 2, NULL }; regmatch_t *prev_idx_match; bool prev_idx_match_malloced = false; #ifdef DEBUG assert (nmatch > 1); assert (mctx->state_log != NULL); #endif if (fl_backtrack) { fs = &fs_body; fs->stack = re_malloc (struct re_fail_stack_ent_t, fs->alloc); if (fs->stack == NULL) return REG_ESPACE; } else fs = NULL; cur_node = dfa->init_node; re_node_set_init_empty (&eps_via_nodes); if (__libc_use_alloca (nmatch * sizeof (regmatch_t))) prev_idx_match = (regmatch_t *) alloca (nmatch * sizeof (regmatch_t)); else { prev_idx_match = re_malloc (regmatch_t, nmatch); if (prev_idx_match == NULL) { free_fail_stack_return (fs); return REG_ESPACE; } prev_idx_match_malloced = true; } memcpy (prev_idx_match, pmatch, sizeof (regmatch_t) * nmatch); for (idx = pmatch[0].rm_so; idx <= pmatch[0].rm_eo ;) { update_regs (dfa, pmatch, prev_idx_match, cur_node, idx, nmatch); if (idx == pmatch[0].rm_eo && cur_node == mctx->last_node) { Idx reg_idx; if (fs) { for (reg_idx = 0; reg_idx < nmatch; ++reg_idx) if (pmatch[reg_idx].rm_so > -1 && pmatch[reg_idx].rm_eo == -1) break; if (reg_idx == nmatch) { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return free_fail_stack_return (fs); } cur_node = pop_fail_stack (fs, &idx, nmatch, pmatch, &eps_via_nodes); } else { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return REG_NOERROR; } } /* Proceed to next node. */ cur_node = proceed_next_node (mctx, nmatch, pmatch, &idx, cur_node, &eps_via_nodes, fs); if (BE (cur_node < 0, 0)) { if (BE (cur_node == -2, 0)) { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); free_fail_stack_return (fs); return REG_ESPACE; } if (fs) cur_node = pop_fail_stack (fs, &idx, nmatch, pmatch, &eps_via_nodes); else { re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return REG_NOMATCH; } } } re_node_set_free (&eps_via_nodes); if (prev_idx_match_malloced) re_free (prev_idx_match); return free_fail_stack_return (fs); } static reg_errcode_t free_fail_stack_return (struct re_fail_stack_t *fs) { if (fs) { Idx fs_idx; for (fs_idx = 0; fs_idx < fs->num; ++fs_idx) { re_node_set_free (&fs->stack[fs_idx].eps_via_nodes); re_free (fs->stack[fs_idx].regs); } re_free (fs->stack); } return REG_NOERROR; } static void update_regs (const re_dfa_t *dfa, regmatch_t *pmatch, regmatch_t *prev_idx_match, Idx cur_node, Idx cur_idx, Idx nmatch) { int type = dfa->nodes[cur_node].type; if (type == OP_OPEN_SUBEXP) { Idx reg_num = dfa->nodes[cur_node].opr.idx + 1; /* We are at the first node of this sub expression. */ if (reg_num < nmatch) { pmatch[reg_num].rm_so = cur_idx; pmatch[reg_num].rm_eo = -1; } } else if (type == OP_CLOSE_SUBEXP) { Idx reg_num = dfa->nodes[cur_node].opr.idx + 1; if (reg_num < nmatch) { /* We are at the last node of this sub expression. */ if (pmatch[reg_num].rm_so < cur_idx) { pmatch[reg_num].rm_eo = cur_idx; /* This is a non-empty match or we are not inside an optional subexpression. Accept this right away. */ memcpy (prev_idx_match, pmatch, sizeof (regmatch_t) * nmatch); } else { if (dfa->nodes[cur_node].opt_subexp && prev_idx_match[reg_num].rm_so != -1) /* We transited through an empty match for an optional subexpression, like (a?)*, and this is not the subexp's first match. Copy back the old content of the registers so that matches of an inner subexpression are undone as well, like in ((a?))*. */ memcpy (pmatch, prev_idx_match, sizeof (regmatch_t) * nmatch); else /* We completed a subexpression, but it may be part of an optional one, so do not update PREV_IDX_MATCH. */ pmatch[reg_num].rm_eo = cur_idx; } } } } /* This function checks the STATE_LOG from the SCTX->last_str_idx to 0 and sift the nodes in each states according to the following rules. Updated state_log will be wrote to STATE_LOG. Rules: We throw away the Node 'a' in the STATE_LOG[STR_IDX] if... 1. When STR_IDX == MATCH_LAST(the last index in the state_log): If 'a' isn't the LAST_NODE and 'a' can't epsilon transit to the LAST_NODE, we throw away the node 'a'. 2. When 0 <= STR_IDX < MATCH_LAST and 'a' accepts string 's' and transit to 'b': i. If 'b' isn't in the STATE_LOG[STR_IDX+strlen('s')], we throw away the node 'a'. ii. If 'b' is in the STATE_LOG[STR_IDX+strlen('s')] but 'b' is thrown away, we throw away the node 'a'. 3. When 0 <= STR_IDX < MATCH_LAST and 'a' epsilon transit to 'b': i. If 'b' isn't in the STATE_LOG[STR_IDX], we throw away the node 'a'. ii. If 'b' is in the STATE_LOG[STR_IDX] but 'b' is thrown away, we throw away the node 'a'. */ #define STATE_NODE_CONTAINS(state,node) \ ((state) != NULL && re_node_set_contains (&(state)->nodes, node)) static reg_errcode_t sift_states_backward (const re_match_context_t *mctx, re_sift_context_t *sctx) { reg_errcode_t err; int null_cnt = 0; Idx str_idx = sctx->last_str_idx; re_node_set cur_dest; #ifdef DEBUG assert (mctx->state_log != NULL && mctx->state_log[str_idx] != NULL); #endif /* Build sifted state_log[str_idx]. It has the nodes which can epsilon transit to the last_node and the last_node itself. */ err = re_node_set_init_1 (&cur_dest, sctx->last_node); if (BE (err != REG_NOERROR, 0)) return err; err = update_cur_sifted_state (mctx, sctx, str_idx, &cur_dest); if (BE (err != REG_NOERROR, 0)) goto free_return; /* Then check each states in the state_log. */ while (str_idx > 0) { /* Update counters. */ null_cnt = (sctx->sifted_states[str_idx] == NULL) ? null_cnt + 1 : 0; if (null_cnt > mctx->max_mb_elem_len) { memset (sctx->sifted_states, '\0', sizeof (re_dfastate_t *) * str_idx); re_node_set_free (&cur_dest); return REG_NOERROR; } re_node_set_empty (&cur_dest); --str_idx; if (mctx->state_log[str_idx]) { err = build_sifted_states (mctx, sctx, str_idx, &cur_dest); if (BE (err != REG_NOERROR, 0)) goto free_return; } /* Add all the nodes which satisfy the following conditions: - It can epsilon transit to a node in CUR_DEST. - It is in CUR_SRC. And update state_log. */ err = update_cur_sifted_state (mctx, sctx, str_idx, &cur_dest); if (BE (err != REG_NOERROR, 0)) goto free_return; } err = REG_NOERROR; free_return: re_node_set_free (&cur_dest); return err; } static reg_errcode_t __attribute_warn_unused_result__ build_sifted_states (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *cur_dest) { const re_dfa_t *const dfa = mctx->dfa; const re_node_set *cur_src = &mctx->state_log[str_idx]->non_eps_nodes; Idx i; /* Then build the next sifted state. We build the next sifted state on 'cur_dest', and update 'sifted_states[str_idx]' with 'cur_dest'. Note: 'cur_dest' is the sifted state from 'state_log[str_idx + 1]'. 'cur_src' points the node_set of the old 'state_log[str_idx]' (with the epsilon nodes pre-filtered out). */ for (i = 0; i < cur_src->nelem; i++) { Idx prev_node = cur_src->elems[i]; int naccepted = 0; bool ok; #ifdef DEBUG re_token_type_t type = dfa->nodes[prev_node].type; assert (!IS_EPSILON_NODE (type)); #endif #ifdef RE_ENABLE_I18N /* If the node may accept "multi byte". */ if (dfa->nodes[prev_node].accept_mb) naccepted = sift_states_iter_mb (mctx, sctx, prev_node, str_idx, sctx->last_str_idx); #endif /* RE_ENABLE_I18N */ /* We don't check backreferences here. See update_cur_sifted_state(). */ if (!naccepted && check_node_accept (mctx, dfa->nodes + prev_node, str_idx) && STATE_NODE_CONTAINS (sctx->sifted_states[str_idx + 1], dfa->nexts[prev_node])) naccepted = 1; if (naccepted == 0) continue; if (sctx->limits.nelem) { Idx to_idx = str_idx + naccepted; if (check_dst_limits (mctx, &sctx->limits, dfa->nexts[prev_node], to_idx, prev_node, str_idx)) continue; } ok = re_node_set_insert (cur_dest, prev_node); if (BE (! ok, 0)) return REG_ESPACE; } return REG_NOERROR; } /* Helper functions. */ static reg_errcode_t clean_state_log_if_needed (re_match_context_t *mctx, Idx next_state_log_idx) { Idx top = mctx->state_log_top; if ((next_state_log_idx >= mctx->input.bufs_len && mctx->input.bufs_len < mctx->input.len) || (next_state_log_idx >= mctx->input.valid_len && mctx->input.valid_len < mctx->input.len)) { reg_errcode_t err; err = extend_buffers (mctx, next_state_log_idx + 1); if (BE (err != REG_NOERROR, 0)) return err; } if (top < next_state_log_idx) { memset (mctx->state_log + top + 1, '\0', sizeof (re_dfastate_t *) * (next_state_log_idx - top)); mctx->state_log_top = next_state_log_idx; } return REG_NOERROR; } static reg_errcode_t merge_state_array (const re_dfa_t *dfa, re_dfastate_t **dst, re_dfastate_t **src, Idx num) { Idx st_idx; reg_errcode_t err; for (st_idx = 0; st_idx < num; ++st_idx) { if (dst[st_idx] == NULL) dst[st_idx] = src[st_idx]; else if (src[st_idx] != NULL) { re_node_set merged_set; err = re_node_set_init_union (&merged_set, &dst[st_idx]->nodes, &src[st_idx]->nodes); if (BE (err != REG_NOERROR, 0)) return err; dst[st_idx] = re_acquire_state (&err, dfa, &merged_set); re_node_set_free (&merged_set); if (BE (err != REG_NOERROR, 0)) return err; } } return REG_NOERROR; } static reg_errcode_t update_cur_sifted_state (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, re_node_set *dest_nodes) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err = REG_NOERROR; const re_node_set *candidates; candidates = ((mctx->state_log[str_idx] == NULL) ? NULL : &mctx->state_log[str_idx]->nodes); if (dest_nodes->nelem == 0) sctx->sifted_states[str_idx] = NULL; else { if (candidates) { /* At first, add the nodes which can epsilon transit to a node in DEST_NODE. */ err = add_epsilon_src_nodes (dfa, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; /* Then, check the limitations in the current sift_context. */ if (sctx->limits.nelem) { err = check_subexp_limits (dfa, dest_nodes, candidates, &sctx->limits, mctx->bkref_ents, str_idx); if (BE (err != REG_NOERROR, 0)) return err; } } sctx->sifted_states[str_idx] = re_acquire_state (&err, dfa, dest_nodes); if (BE (err != REG_NOERROR, 0)) return err; } if (candidates && mctx->state_log[str_idx]->has_backref) { err = sift_states_bkref (mctx, sctx, str_idx, candidates); if (BE (err != REG_NOERROR, 0)) return err; } return REG_NOERROR; } static reg_errcode_t __attribute_warn_unused_result__ add_epsilon_src_nodes (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates) { reg_errcode_t err = REG_NOERROR; Idx i; re_dfastate_t *state = re_acquire_state (&err, dfa, dest_nodes); if (BE (err != REG_NOERROR, 0)) return err; if (!state->inveclosure.alloc) { err = re_node_set_alloc (&state->inveclosure, dest_nodes->nelem); if (BE (err != REG_NOERROR, 0)) return REG_ESPACE; for (i = 0; i < dest_nodes->nelem; i++) { err = re_node_set_merge (&state->inveclosure, dfa->inveclosures + dest_nodes->elems[i]); if (BE (err != REG_NOERROR, 0)) return REG_ESPACE; } } return re_node_set_add_intersect (dest_nodes, candidates, &state->inveclosure); } static reg_errcode_t sub_epsilon_src_nodes (const re_dfa_t *dfa, Idx node, re_node_set *dest_nodes, const re_node_set *candidates) { Idx ecl_idx; reg_errcode_t err; re_node_set *inv_eclosure = dfa->inveclosures + node; re_node_set except_nodes; re_node_set_init_empty (&except_nodes); for (ecl_idx = 0; ecl_idx < inv_eclosure->nelem; ++ecl_idx) { Idx cur_node = inv_eclosure->elems[ecl_idx]; if (cur_node == node) continue; if (IS_EPSILON_NODE (dfa->nodes[cur_node].type)) { Idx edst1 = dfa->edests[cur_node].elems[0]; Idx edst2 = ((dfa->edests[cur_node].nelem > 1) ? dfa->edests[cur_node].elems[1] : -1); if ((!re_node_set_contains (inv_eclosure, edst1) && re_node_set_contains (dest_nodes, edst1)) || (edst2 > 0 && !re_node_set_contains (inv_eclosure, edst2) && re_node_set_contains (dest_nodes, edst2))) { err = re_node_set_add_intersect (&except_nodes, candidates, dfa->inveclosures + cur_node); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&except_nodes); return err; } } } } for (ecl_idx = 0; ecl_idx < inv_eclosure->nelem; ++ecl_idx) { Idx cur_node = inv_eclosure->elems[ecl_idx]; if (!re_node_set_contains (&except_nodes, cur_node)) { Idx idx = re_node_set_contains (dest_nodes, cur_node) - 1; re_node_set_remove_at (dest_nodes, idx); } } re_node_set_free (&except_nodes); return REG_NOERROR; } static bool check_dst_limits (const re_match_context_t *mctx, const re_node_set *limits, Idx dst_node, Idx dst_idx, Idx src_node, Idx src_idx) { const re_dfa_t *const dfa = mctx->dfa; Idx lim_idx, src_pos, dst_pos; Idx dst_bkref_idx = search_cur_bkref_entry (mctx, dst_idx); Idx src_bkref_idx = search_cur_bkref_entry (mctx, src_idx); for (lim_idx = 0; lim_idx < limits->nelem; ++lim_idx) { Idx subexp_idx; struct re_backref_cache_entry *ent; ent = mctx->bkref_ents + limits->elems[lim_idx]; subexp_idx = dfa->nodes[ent->node].opr.idx; dst_pos = check_dst_limits_calc_pos (mctx, limits->elems[lim_idx], subexp_idx, dst_node, dst_idx, dst_bkref_idx); src_pos = check_dst_limits_calc_pos (mctx, limits->elems[lim_idx], subexp_idx, src_node, src_idx, src_bkref_idx); /* In case of: ( ) ( ) ( ) */ if (src_pos == dst_pos) continue; /* This is unrelated limitation. */ else return true; } return false; } static int check_dst_limits_calc_pos_1 (const re_match_context_t *mctx, int boundaries, Idx subexp_idx, Idx from_node, Idx bkref_idx) { const re_dfa_t *const dfa = mctx->dfa; const re_node_set *eclosures = dfa->eclosures + from_node; Idx node_idx; /* Else, we are on the boundary: examine the nodes on the epsilon closure. */ for (node_idx = 0; node_idx < eclosures->nelem; ++node_idx) { Idx node = eclosures->elems[node_idx]; switch (dfa->nodes[node].type) { case OP_BACK_REF: if (bkref_idx != -1) { struct re_backref_cache_entry *ent = mctx->bkref_ents + bkref_idx; do { Idx dst; int cpos; if (ent->node != node) continue; if (subexp_idx < BITSET_WORD_BITS && !(ent->eps_reachable_subexps_map & ((bitset_word_t) 1 << subexp_idx))) continue; /* Recurse trying to reach the OP_OPEN_SUBEXP and OP_CLOSE_SUBEXP cases below. But, if the destination node is the same node as the source node, don't recurse because it would cause an infinite loop: a regex that exhibits this behavior is ()\1*\1* */ dst = dfa->edests[node].elems[0]; if (dst == from_node) { if (boundaries & 1) return -1; else /* if (boundaries & 2) */ return 0; } cpos = check_dst_limits_calc_pos_1 (mctx, boundaries, subexp_idx, dst, bkref_idx); if (cpos == -1 /* && (boundaries & 1) */) return -1; if (cpos == 0 && (boundaries & 2)) return 0; if (subexp_idx < BITSET_WORD_BITS) ent->eps_reachable_subexps_map &= ~((bitset_word_t) 1 << subexp_idx); } while (ent++->more); } break; case OP_OPEN_SUBEXP: if ((boundaries & 1) && subexp_idx == dfa->nodes[node].opr.idx) return -1; break; case OP_CLOSE_SUBEXP: if ((boundaries & 2) && subexp_idx == dfa->nodes[node].opr.idx) return 0; break; default: break; } } return (boundaries & 2) ? 1 : 0; } static int check_dst_limits_calc_pos (const re_match_context_t *mctx, Idx limit, Idx subexp_idx, Idx from_node, Idx str_idx, Idx bkref_idx) { struct re_backref_cache_entry *lim = mctx->bkref_ents + limit; int boundaries; /* If we are outside the range of the subexpression, return -1 or 1. */ if (str_idx < lim->subexp_from) return -1; if (lim->subexp_to < str_idx) return 1; /* If we are within the subexpression, return 0. */ boundaries = (str_idx == lim->subexp_from); boundaries |= (str_idx == lim->subexp_to) << 1; if (boundaries == 0) return 0; /* Else, examine epsilon closure. */ return check_dst_limits_calc_pos_1 (mctx, boundaries, subexp_idx, from_node, bkref_idx); } /* Check the limitations of sub expressions LIMITS, and remove the nodes which are against limitations from DEST_NODES. */ static reg_errcode_t check_subexp_limits (const re_dfa_t *dfa, re_node_set *dest_nodes, const re_node_set *candidates, re_node_set *limits, struct re_backref_cache_entry *bkref_ents, Idx str_idx) { reg_errcode_t err; Idx node_idx, lim_idx; for (lim_idx = 0; lim_idx < limits->nelem; ++lim_idx) { Idx subexp_idx; struct re_backref_cache_entry *ent; ent = bkref_ents + limits->elems[lim_idx]; if (str_idx <= ent->subexp_from || ent->str_idx < str_idx) continue; /* This is unrelated limitation. */ subexp_idx = dfa->nodes[ent->node].opr.idx; if (ent->subexp_to == str_idx) { Idx ops_node = -1; Idx cls_node = -1; for (node_idx = 0; node_idx < dest_nodes->nelem; ++node_idx) { Idx node = dest_nodes->elems[node_idx]; re_token_type_t type = dfa->nodes[node].type; if (type == OP_OPEN_SUBEXP && subexp_idx == dfa->nodes[node].opr.idx) ops_node = node; else if (type == OP_CLOSE_SUBEXP && subexp_idx == dfa->nodes[node].opr.idx) cls_node = node; } /* Check the limitation of the open subexpression. */ /* Note that (ent->subexp_to = str_idx != ent->subexp_from). */ if (ops_node >= 0) { err = sub_epsilon_src_nodes (dfa, ops_node, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; } /* Check the limitation of the close subexpression. */ if (cls_node >= 0) for (node_idx = 0; node_idx < dest_nodes->nelem; ++node_idx) { Idx node = dest_nodes->elems[node_idx]; if (!re_node_set_contains (dfa->inveclosures + node, cls_node) && !re_node_set_contains (dfa->eclosures + node, cls_node)) { /* It is against this limitation. Remove it form the current sifted state. */ err = sub_epsilon_src_nodes (dfa, node, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; --node_idx; } } } else /* (ent->subexp_to != str_idx) */ { for (node_idx = 0; node_idx < dest_nodes->nelem; ++node_idx) { Idx node = dest_nodes->elems[node_idx]; re_token_type_t type = dfa->nodes[node].type; if (type == OP_CLOSE_SUBEXP || type == OP_OPEN_SUBEXP) { if (subexp_idx != dfa->nodes[node].opr.idx) continue; /* It is against this limitation. Remove it form the current sifted state. */ err = sub_epsilon_src_nodes (dfa, node, dest_nodes, candidates); if (BE (err != REG_NOERROR, 0)) return err; } } } } return REG_NOERROR; } static reg_errcode_t __attribute_warn_unused_result__ sift_states_bkref (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx str_idx, const re_node_set *candidates) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx node_idx, node; re_sift_context_t local_sctx; Idx first_idx = search_cur_bkref_entry (mctx, str_idx); if (first_idx == -1) return REG_NOERROR; local_sctx.sifted_states = NULL; /* Mark that it hasn't been initialized. */ for (node_idx = 0; node_idx < candidates->nelem; ++node_idx) { Idx enabled_idx; re_token_type_t type; struct re_backref_cache_entry *entry; node = candidates->elems[node_idx]; type = dfa->nodes[node].type; /* Avoid infinite loop for the REs like "()\1+". */ if (node == sctx->last_node && str_idx == sctx->last_str_idx) continue; if (type != OP_BACK_REF) continue; entry = mctx->bkref_ents + first_idx; enabled_idx = first_idx; do { Idx subexp_len; Idx to_idx; Idx dst_node; bool ok; re_dfastate_t *cur_state; if (entry->node != node) continue; subexp_len = entry->subexp_to - entry->subexp_from; to_idx = str_idx + subexp_len; dst_node = (subexp_len ? dfa->nexts[node] : dfa->edests[node].elems[0]); if (to_idx > sctx->last_str_idx || sctx->sifted_states[to_idx] == NULL || !STATE_NODE_CONTAINS (sctx->sifted_states[to_idx], dst_node) || check_dst_limits (mctx, &sctx->limits, node, str_idx, dst_node, to_idx)) continue; if (local_sctx.sifted_states == NULL) { local_sctx = *sctx; err = re_node_set_init_copy (&local_sctx.limits, &sctx->limits); if (BE (err != REG_NOERROR, 0)) goto free_return; } local_sctx.last_node = node; local_sctx.last_str_idx = str_idx; ok = re_node_set_insert (&local_sctx.limits, enabled_idx); if (BE (! ok, 0)) { err = REG_ESPACE; goto free_return; } cur_state = local_sctx.sifted_states[str_idx]; err = sift_states_backward (mctx, &local_sctx); if (BE (err != REG_NOERROR, 0)) goto free_return; if (sctx->limited_states != NULL) { err = merge_state_array (dfa, sctx->limited_states, local_sctx.sifted_states, str_idx + 1); if (BE (err != REG_NOERROR, 0)) goto free_return; } local_sctx.sifted_states[str_idx] = cur_state; re_node_set_remove (&local_sctx.limits, enabled_idx); /* mctx->bkref_ents may have changed, reload the pointer. */ entry = mctx->bkref_ents + enabled_idx; } while (enabled_idx++, entry++->more); } err = REG_NOERROR; free_return: if (local_sctx.sifted_states != NULL) { re_node_set_free (&local_sctx.limits); } return err; } #ifdef RE_ENABLE_I18N static int sift_states_iter_mb (const re_match_context_t *mctx, re_sift_context_t *sctx, Idx node_idx, Idx str_idx, Idx max_str_idx) { const re_dfa_t *const dfa = mctx->dfa; int naccepted; /* Check the node can accept "multi byte". */ naccepted = check_node_accept_bytes (dfa, node_idx, &mctx->input, str_idx); if (naccepted > 0 && str_idx + naccepted <= max_str_idx && !STATE_NODE_CONTAINS (sctx->sifted_states[str_idx + naccepted], dfa->nexts[node_idx])) /* The node can't accept the "multi byte", or the destination was already thrown away, then the node could't accept the current input "multi byte". */ naccepted = 0; /* Otherwise, it is sure that the node could accept 'naccepted' bytes input. */ return naccepted; } #endif /* RE_ENABLE_I18N */ /* Functions for state transition. */ /* Return the next state to which the current state STATE will transit by accepting the current input byte, and update STATE_LOG if necessary. If STATE can accept a multibyte char/collating element/back reference update the destination of STATE_LOG. */ static re_dfastate_t * __attribute_warn_unused_result__ transit_state (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *state) { re_dfastate_t **trtable; unsigned char ch; #ifdef RE_ENABLE_I18N /* If the current state can accept multibyte. */ if (BE (state->accept_mb, 0)) { *err = transit_state_mb (mctx, state); if (BE (*err != REG_NOERROR, 0)) return NULL; } #endif /* RE_ENABLE_I18N */ /* Then decide the next state with the single byte. */ #if 0 if (0) /* don't use transition table */ return transit_state_sb (err, mctx, state); #endif /* Use transition table */ ch = re_string_fetch_byte (&mctx->input); for (;;) { trtable = state->trtable; if (BE (trtable != NULL, 1)) return trtable[ch]; trtable = state->word_trtable; if (BE (trtable != NULL, 1)) { unsigned int context; context = re_string_context_at (&mctx->input, re_string_cur_idx (&mctx->input) - 1, mctx->eflags); if (IS_WORD_CONTEXT (context)) return trtable[ch + SBC_MAX]; else return trtable[ch]; } if (!build_trtable (mctx->dfa, state)) { *err = REG_ESPACE; return NULL; } /* Retry, we now have a transition table. */ } } /* Update the state_log if we need */ static re_dfastate_t * merge_state_with_log (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *next_state) { const re_dfa_t *const dfa = mctx->dfa; Idx cur_idx = re_string_cur_idx (&mctx->input); if (cur_idx > mctx->state_log_top) { mctx->state_log[cur_idx] = next_state; mctx->state_log_top = cur_idx; } else if (mctx->state_log[cur_idx] == 0) { mctx->state_log[cur_idx] = next_state; } else { re_dfastate_t *pstate; unsigned int context; re_node_set next_nodes, *log_nodes, *table_nodes = NULL; /* If (state_log[cur_idx] != 0), it implies that cur_idx is the destination of a multibyte char/collating element/ back reference. Then the next state is the union set of these destinations and the results of the transition table. */ pstate = mctx->state_log[cur_idx]; log_nodes = pstate->entrance_nodes; if (next_state != NULL) { table_nodes = next_state->entrance_nodes; *err = re_node_set_init_union (&next_nodes, table_nodes, log_nodes); if (BE (*err != REG_NOERROR, 0)) return NULL; } else next_nodes = *log_nodes; /* Note: We already add the nodes of the initial state, then we don't need to add them here. */ context = re_string_context_at (&mctx->input, re_string_cur_idx (&mctx->input) - 1, mctx->eflags); next_state = mctx->state_log[cur_idx] = re_acquire_state_context (err, dfa, &next_nodes, context); /* We don't need to check errors here, since the return value of this function is next_state and ERR is already set. */ if (table_nodes != NULL) re_node_set_free (&next_nodes); } if (BE (dfa->nbackref, 0) && next_state != NULL) { /* Check OP_OPEN_SUBEXP in the current state in case that we use them later. We must check them here, since the back references in the next state might use them. */ *err = check_subexp_matching_top (mctx, &next_state->nodes, cur_idx); if (BE (*err != REG_NOERROR, 0)) return NULL; /* If the next state has back references. */ if (next_state->has_backref) { *err = transit_state_bkref (mctx, &next_state->nodes); if (BE (*err != REG_NOERROR, 0)) return NULL; next_state = mctx->state_log[cur_idx]; } } return next_state; } /* Skip bytes in the input that correspond to part of a multi-byte match, then look in the log for a state from which to restart matching. */ static re_dfastate_t * find_recover_state (reg_errcode_t *err, re_match_context_t *mctx) { re_dfastate_t *cur_state; do { Idx max = mctx->state_log_top; Idx cur_str_idx = re_string_cur_idx (&mctx->input); do { if (++cur_str_idx > max) return NULL; re_string_skip_bytes (&mctx->input, 1); } while (mctx->state_log[cur_str_idx] == NULL); cur_state = merge_state_with_log (err, mctx, NULL); } while (*err == REG_NOERROR && cur_state == NULL); return cur_state; } /* Helper functions for transit_state. */ /* From the node set CUR_NODES, pick up the nodes whose types are OP_OPEN_SUBEXP and which have corresponding back references in the regular expression. And register them to use them later for evaluating the corresponding back references. */ static reg_errcode_t check_subexp_matching_top (re_match_context_t *mctx, re_node_set *cur_nodes, Idx str_idx) { const re_dfa_t *const dfa = mctx->dfa; Idx node_idx; reg_errcode_t err; /* TODO: This isn't efficient. Because there might be more than one nodes whose types are OP_OPEN_SUBEXP and whose index is SUBEXP_IDX, we must check all nodes. E.g. RE: (a){2} */ for (node_idx = 0; node_idx < cur_nodes->nelem; ++node_idx) { Idx node = cur_nodes->elems[node_idx]; if (dfa->nodes[node].type == OP_OPEN_SUBEXP && dfa->nodes[node].opr.idx < BITSET_WORD_BITS && (dfa->used_bkref_map & ((bitset_word_t) 1 << dfa->nodes[node].opr.idx))) { err = match_ctx_add_subtop (mctx, node, str_idx); if (BE (err != REG_NOERROR, 0)) return err; } } return REG_NOERROR; } #if 0 /* Return the next state to which the current state STATE will transit by accepting the current input byte. */ static re_dfastate_t * transit_state_sb (reg_errcode_t *err, re_match_context_t *mctx, re_dfastate_t *state) { const re_dfa_t *const dfa = mctx->dfa; re_node_set next_nodes; re_dfastate_t *next_state; Idx node_cnt, cur_str_idx = re_string_cur_idx (&mctx->input); unsigned int context; *err = re_node_set_alloc (&next_nodes, state->nodes.nelem + 1); if (BE (*err != REG_NOERROR, 0)) return NULL; for (node_cnt = 0; node_cnt < state->nodes.nelem; ++node_cnt) { Idx cur_node = state->nodes.elems[node_cnt]; if (check_node_accept (mctx, dfa->nodes + cur_node, cur_str_idx)) { *err = re_node_set_merge (&next_nodes, dfa->eclosures + dfa->nexts[cur_node]); if (BE (*err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return NULL; } } } context = re_string_context_at (&mctx->input, cur_str_idx, mctx->eflags); next_state = re_acquire_state_context (err, dfa, &next_nodes, context); /* We don't need to check errors here, since the return value of this function is next_state and ERR is already set. */ re_node_set_free (&next_nodes); re_string_skip_bytes (&mctx->input, 1); return next_state; } #endif #ifdef RE_ENABLE_I18N static reg_errcode_t transit_state_mb (re_match_context_t *mctx, re_dfastate_t *pstate) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx i; for (i = 0; i < pstate->nodes.nelem; ++i) { re_node_set dest_nodes, *new_nodes; Idx cur_node_idx = pstate->nodes.elems[i]; int naccepted; Idx dest_idx; unsigned int context; re_dfastate_t *dest_state; if (!dfa->nodes[cur_node_idx].accept_mb) continue; if (dfa->nodes[cur_node_idx].constraint) { context = re_string_context_at (&mctx->input, re_string_cur_idx (&mctx->input), mctx->eflags); if (NOT_SATISFY_NEXT_CONSTRAINT (dfa->nodes[cur_node_idx].constraint, context)) continue; } /* How many bytes the node can accept? */ naccepted = check_node_accept_bytes (dfa, cur_node_idx, &mctx->input, re_string_cur_idx (&mctx->input)); if (naccepted == 0) continue; /* The node can accepts 'naccepted' bytes. */ dest_idx = re_string_cur_idx (&mctx->input) + naccepted; mctx->max_mb_elem_len = ((mctx->max_mb_elem_len < naccepted) ? naccepted : mctx->max_mb_elem_len); err = clean_state_log_if_needed (mctx, dest_idx); if (BE (err != REG_NOERROR, 0)) return err; #ifdef DEBUG assert (dfa->nexts[cur_node_idx] != -1); #endif new_nodes = dfa->eclosures + dfa->nexts[cur_node_idx]; dest_state = mctx->state_log[dest_idx]; if (dest_state == NULL) dest_nodes = *new_nodes; else { err = re_node_set_init_union (&dest_nodes, dest_state->entrance_nodes, new_nodes); if (BE (err != REG_NOERROR, 0)) return err; } context = re_string_context_at (&mctx->input, dest_idx - 1, mctx->eflags); mctx->state_log[dest_idx] = re_acquire_state_context (&err, dfa, &dest_nodes, context); if (dest_state != NULL) re_node_set_free (&dest_nodes); if (BE (mctx->state_log[dest_idx] == NULL && err != REG_NOERROR, 0)) return err; } return REG_NOERROR; } #endif /* RE_ENABLE_I18N */ static reg_errcode_t transit_state_bkref (re_match_context_t *mctx, const re_node_set *nodes) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx i; Idx cur_str_idx = re_string_cur_idx (&mctx->input); for (i = 0; i < nodes->nelem; ++i) { Idx dest_str_idx, prev_nelem, bkc_idx; Idx node_idx = nodes->elems[i]; unsigned int context; const re_token_t *node = dfa->nodes + node_idx; re_node_set *new_dest_nodes; /* Check whether 'node' is a backreference or not. */ if (node->type != OP_BACK_REF) continue; if (node->constraint) { context = re_string_context_at (&mctx->input, cur_str_idx, mctx->eflags); if (NOT_SATISFY_NEXT_CONSTRAINT (node->constraint, context)) continue; } /* 'node' is a backreference. Check the substring which the substring matched. */ bkc_idx = mctx->nbkref_ents; err = get_subexp (mctx, node_idx, cur_str_idx); if (BE (err != REG_NOERROR, 0)) goto free_return; /* And add the epsilon closures (which is 'new_dest_nodes') of the backreference to appropriate state_log. */ #ifdef DEBUG assert (dfa->nexts[node_idx] != -1); #endif for (; bkc_idx < mctx->nbkref_ents; ++bkc_idx) { Idx subexp_len; re_dfastate_t *dest_state; struct re_backref_cache_entry *bkref_ent; bkref_ent = mctx->bkref_ents + bkc_idx; if (bkref_ent->node != node_idx || bkref_ent->str_idx != cur_str_idx) continue; subexp_len = bkref_ent->subexp_to - bkref_ent->subexp_from; new_dest_nodes = (subexp_len == 0 ? dfa->eclosures + dfa->edests[node_idx].elems[0] : dfa->eclosures + dfa->nexts[node_idx]); dest_str_idx = (cur_str_idx + bkref_ent->subexp_to - bkref_ent->subexp_from); context = re_string_context_at (&mctx->input, dest_str_idx - 1, mctx->eflags); dest_state = mctx->state_log[dest_str_idx]; prev_nelem = ((mctx->state_log[cur_str_idx] == NULL) ? 0 : mctx->state_log[cur_str_idx]->nodes.nelem); /* Add 'new_dest_node' to state_log. */ if (dest_state == NULL) { mctx->state_log[dest_str_idx] = re_acquire_state_context (&err, dfa, new_dest_nodes, context); if (BE (mctx->state_log[dest_str_idx] == NULL && err != REG_NOERROR, 0)) goto free_return; } else { re_node_set dest_nodes; err = re_node_set_init_union (&dest_nodes, dest_state->entrance_nodes, new_dest_nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&dest_nodes); goto free_return; } mctx->state_log[dest_str_idx] = re_acquire_state_context (&err, dfa, &dest_nodes, context); re_node_set_free (&dest_nodes); if (BE (mctx->state_log[dest_str_idx] == NULL && err != REG_NOERROR, 0)) goto free_return; } /* We need to check recursively if the backreference can epsilon transit. */ if (subexp_len == 0 && mctx->state_log[cur_str_idx]->nodes.nelem > prev_nelem) { err = check_subexp_matching_top (mctx, new_dest_nodes, cur_str_idx); if (BE (err != REG_NOERROR, 0)) goto free_return; err = transit_state_bkref (mctx, new_dest_nodes); if (BE (err != REG_NOERROR, 0)) goto free_return; } } } err = REG_NOERROR; free_return: return err; } /* Enumerate all the candidates which the backreference BKREF_NODE can match at BKREF_STR_IDX, and register them by match_ctx_add_entry(). Note that we might collect inappropriate candidates here. However, the cost of checking them strictly here is too high, then we delay these checking for prune_impossible_nodes(). */ static reg_errcode_t __attribute_warn_unused_result__ get_subexp (re_match_context_t *mctx, Idx bkref_node, Idx bkref_str_idx) { const re_dfa_t *const dfa = mctx->dfa; Idx subexp_num, sub_top_idx; const char *buf = (const char *) re_string_get_buffer (&mctx->input); /* Return if we have already checked BKREF_NODE at BKREF_STR_IDX. */ Idx cache_idx = search_cur_bkref_entry (mctx, bkref_str_idx); if (cache_idx != -1) { const struct re_backref_cache_entry *entry = mctx->bkref_ents + cache_idx; do if (entry->node == bkref_node) return REG_NOERROR; /* We already checked it. */ while (entry++->more); } subexp_num = dfa->nodes[bkref_node].opr.idx; /* For each sub expression */ for (sub_top_idx = 0; sub_top_idx < mctx->nsub_tops; ++sub_top_idx) { reg_errcode_t err; re_sub_match_top_t *sub_top = mctx->sub_tops[sub_top_idx]; re_sub_match_last_t *sub_last; Idx sub_last_idx, sl_str, bkref_str_off; if (dfa->nodes[sub_top->node].opr.idx != subexp_num) continue; /* It isn't related. */ sl_str = sub_top->str_idx; bkref_str_off = bkref_str_idx; /* At first, check the last node of sub expressions we already evaluated. */ for (sub_last_idx = 0; sub_last_idx < sub_top->nlasts; ++sub_last_idx) { regoff_t sl_str_diff; sub_last = sub_top->lasts[sub_last_idx]; sl_str_diff = sub_last->str_idx - sl_str; /* The matched string by the sub expression match with the substring at the back reference? */ if (sl_str_diff > 0) { if (BE (bkref_str_off + sl_str_diff > mctx->input.valid_len, 0)) { /* Not enough chars for a successful match. */ if (bkref_str_off + sl_str_diff > mctx->input.len) break; err = clean_state_log_if_needed (mctx, bkref_str_off + sl_str_diff); if (BE (err != REG_NOERROR, 0)) return err; buf = (const char *) re_string_get_buffer (&mctx->input); } if (memcmp (buf + bkref_str_off, buf + sl_str, sl_str_diff) != 0) /* We don't need to search this sub expression any more. */ break; } bkref_str_off += sl_str_diff; sl_str += sl_str_diff; err = get_subexp_sub (mctx, sub_top, sub_last, bkref_node, bkref_str_idx); /* Reload buf, since the preceding call might have reallocated the buffer. */ buf = (const char *) re_string_get_buffer (&mctx->input); if (err == REG_NOMATCH) continue; if (BE (err != REG_NOERROR, 0)) return err; } if (sub_last_idx < sub_top->nlasts) continue; if (sub_last_idx > 0) ++sl_str; /* Then, search for the other last nodes of the sub expression. */ for (; sl_str <= bkref_str_idx; ++sl_str) { Idx cls_node; regoff_t sl_str_off; const re_node_set *nodes; sl_str_off = sl_str - sub_top->str_idx; /* The matched string by the sub expression match with the substring at the back reference? */ if (sl_str_off > 0) { if (BE (bkref_str_off >= mctx->input.valid_len, 0)) { /* If we are at the end of the input, we cannot match. */ if (bkref_str_off >= mctx->input.len) break; err = extend_buffers (mctx, bkref_str_off + 1); if (BE (err != REG_NOERROR, 0)) return err; buf = (const char *) re_string_get_buffer (&mctx->input); } if (buf [bkref_str_off++] != buf[sl_str - 1]) break; /* We don't need to search this sub expression any more. */ } if (mctx->state_log[sl_str] == NULL) continue; /* Does this state have a ')' of the sub expression? */ nodes = &mctx->state_log[sl_str]->nodes; cls_node = find_subexp_node (dfa, nodes, subexp_num, OP_CLOSE_SUBEXP); if (cls_node == -1) continue; /* No. */ if (sub_top->path == NULL) { sub_top->path = calloc (sizeof (state_array_t), sl_str - sub_top->str_idx + 1); if (sub_top->path == NULL) return REG_ESPACE; } /* Can the OP_OPEN_SUBEXP node arrive the OP_CLOSE_SUBEXP node in the current context? */ err = check_arrival (mctx, sub_top->path, sub_top->node, sub_top->str_idx, cls_node, sl_str, OP_CLOSE_SUBEXP); if (err == REG_NOMATCH) continue; if (BE (err != REG_NOERROR, 0)) return err; sub_last = match_ctx_add_sublast (sub_top, cls_node, sl_str); if (BE (sub_last == NULL, 0)) return REG_ESPACE; err = get_subexp_sub (mctx, sub_top, sub_last, bkref_node, bkref_str_idx); if (err == REG_NOMATCH) continue; } } return REG_NOERROR; } /* Helper functions for get_subexp(). */ /* Check SUB_LAST can arrive to the back reference BKREF_NODE at BKREF_STR. If it can arrive, register the sub expression expressed with SUB_TOP and SUB_LAST. */ static reg_errcode_t get_subexp_sub (re_match_context_t *mctx, const re_sub_match_top_t *sub_top, re_sub_match_last_t *sub_last, Idx bkref_node, Idx bkref_str) { reg_errcode_t err; Idx to_idx; /* Can the subexpression arrive the back reference? */ err = check_arrival (mctx, &sub_last->path, sub_last->node, sub_last->str_idx, bkref_node, bkref_str, OP_OPEN_SUBEXP); if (err != REG_NOERROR) return err; err = match_ctx_add_entry (mctx, bkref_node, bkref_str, sub_top->str_idx, sub_last->str_idx); if (BE (err != REG_NOERROR, 0)) return err; to_idx = bkref_str + sub_last->str_idx - sub_top->str_idx; return clean_state_log_if_needed (mctx, to_idx); } /* Find the first node which is '(' or ')' and whose index is SUBEXP_IDX. Search '(' if FL_OPEN, or search ')' otherwise. TODO: This function isn't efficient... Because there might be more than one nodes whose types are OP_OPEN_SUBEXP and whose index is SUBEXP_IDX, we must check all nodes. E.g. RE: (a){2} */ static Idx find_subexp_node (const re_dfa_t *dfa, const re_node_set *nodes, Idx subexp_idx, int type) { Idx cls_idx; for (cls_idx = 0; cls_idx < nodes->nelem; ++cls_idx) { Idx cls_node = nodes->elems[cls_idx]; const re_token_t *node = dfa->nodes + cls_node; if (node->type == type && node->opr.idx == subexp_idx) return cls_node; } return -1; } /* Check whether the node TOP_NODE at TOP_STR can arrive to the node LAST_NODE at LAST_STR. We record the path onto PATH since it will be heavily reused. Return REG_NOERROR if it can arrive, or REG_NOMATCH otherwise. */ static reg_errcode_t __attribute_warn_unused_result__ check_arrival (re_match_context_t *mctx, state_array_t *path, Idx top_node, Idx top_str, Idx last_node, Idx last_str, int type) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err = REG_NOERROR; Idx subexp_num, backup_cur_idx, str_idx, null_cnt; re_dfastate_t *cur_state = NULL; re_node_set *cur_nodes, next_nodes; re_dfastate_t **backup_state_log; unsigned int context; subexp_num = dfa->nodes[top_node].opr.idx; /* Extend the buffer if we need. */ if (BE (path->alloc < last_str + mctx->max_mb_elem_len + 1, 0)) { re_dfastate_t **new_array; Idx old_alloc = path->alloc; Idx incr_alloc = last_str + mctx->max_mb_elem_len + 1; Idx new_alloc; if (BE (IDX_MAX - old_alloc < incr_alloc, 0)) return REG_ESPACE; new_alloc = old_alloc + incr_alloc; if (BE (SIZE_MAX / sizeof (re_dfastate_t *) < new_alloc, 0)) return REG_ESPACE; new_array = re_realloc (path->array, re_dfastate_t *, new_alloc); if (BE (new_array == NULL, 0)) return REG_ESPACE; path->array = new_array; path->alloc = new_alloc; memset (new_array + old_alloc, '\0', sizeof (re_dfastate_t *) * (path->alloc - old_alloc)); } str_idx = path->next_idx ? path->next_idx : top_str; /* Temporary modify MCTX. */ backup_state_log = mctx->state_log; backup_cur_idx = mctx->input.cur_idx; mctx->state_log = path->array; mctx->input.cur_idx = str_idx; /* Setup initial node set. */ context = re_string_context_at (&mctx->input, str_idx - 1, mctx->eflags); if (str_idx == top_str) { err = re_node_set_init_1 (&next_nodes, top_node); if (BE (err != REG_NOERROR, 0)) return err; err = check_arrival_expand_ecl (dfa, &next_nodes, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } else { cur_state = mctx->state_log[str_idx]; if (cur_state && cur_state->has_backref) { err = re_node_set_init_copy (&next_nodes, &cur_state->nodes); if (BE (err != REG_NOERROR, 0)) return err; } else re_node_set_init_empty (&next_nodes); } if (str_idx == top_str || (cur_state && cur_state->has_backref)) { if (next_nodes.nelem) { err = expand_bkref_cache (mctx, &next_nodes, str_idx, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } cur_state = re_acquire_state_context (&err, dfa, &next_nodes, context); if (BE (cur_state == NULL && err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } mctx->state_log[str_idx] = cur_state; } for (null_cnt = 0; str_idx < last_str && null_cnt <= mctx->max_mb_elem_len;) { re_node_set_empty (&next_nodes); if (mctx->state_log[str_idx + 1]) { err = re_node_set_merge (&next_nodes, &mctx->state_log[str_idx + 1]->nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } if (cur_state) { err = check_arrival_add_next_nodes (mctx, str_idx, &cur_state->non_eps_nodes, &next_nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } ++str_idx; if (next_nodes.nelem) { err = check_arrival_expand_ecl (dfa, &next_nodes, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } err = expand_bkref_cache (mctx, &next_nodes, str_idx, subexp_num, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } } context = re_string_context_at (&mctx->input, str_idx - 1, mctx->eflags); cur_state = re_acquire_state_context (&err, dfa, &next_nodes, context); if (BE (cur_state == NULL && err != REG_NOERROR, 0)) { re_node_set_free (&next_nodes); return err; } mctx->state_log[str_idx] = cur_state; null_cnt = cur_state == NULL ? null_cnt + 1 : 0; } re_node_set_free (&next_nodes); cur_nodes = (mctx->state_log[last_str] == NULL ? NULL : &mctx->state_log[last_str]->nodes); path->next_idx = str_idx; /* Fix MCTX. */ mctx->state_log = backup_state_log; mctx->input.cur_idx = backup_cur_idx; /* Then check the current node set has the node LAST_NODE. */ if (cur_nodes != NULL && re_node_set_contains (cur_nodes, last_node)) return REG_NOERROR; return REG_NOMATCH; } /* Helper functions for check_arrival. */ /* Calculate the destination nodes of CUR_NODES at STR_IDX, and append them to NEXT_NODES. TODO: This function is similar to the functions transit_state*(), however this function has many additional works. Can't we unify them? */ static reg_errcode_t __attribute_warn_unused_result__ check_arrival_add_next_nodes (re_match_context_t *mctx, Idx str_idx, re_node_set *cur_nodes, re_node_set *next_nodes) { const re_dfa_t *const dfa = mctx->dfa; bool ok; Idx cur_idx; #ifdef RE_ENABLE_I18N reg_errcode_t err = REG_NOERROR; #endif re_node_set union_set; re_node_set_init_empty (&union_set); for (cur_idx = 0; cur_idx < cur_nodes->nelem; ++cur_idx) { int naccepted = 0; Idx cur_node = cur_nodes->elems[cur_idx]; #ifdef DEBUG re_token_type_t type = dfa->nodes[cur_node].type; assert (!IS_EPSILON_NODE (type)); #endif #ifdef RE_ENABLE_I18N /* If the node may accept "multi byte". */ if (dfa->nodes[cur_node].accept_mb) { naccepted = check_node_accept_bytes (dfa, cur_node, &mctx->input, str_idx); if (naccepted > 1) { re_dfastate_t *dest_state; Idx next_node = dfa->nexts[cur_node]; Idx next_idx = str_idx + naccepted; dest_state = mctx->state_log[next_idx]; re_node_set_empty (&union_set); if (dest_state) { err = re_node_set_merge (&union_set, &dest_state->nodes); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&union_set); return err; } } ok = re_node_set_insert (&union_set, next_node); if (BE (! ok, 0)) { re_node_set_free (&union_set); return REG_ESPACE; } mctx->state_log[next_idx] = re_acquire_state (&err, dfa, &union_set); if (BE (mctx->state_log[next_idx] == NULL && err != REG_NOERROR, 0)) { re_node_set_free (&union_set); return err; } } } #endif /* RE_ENABLE_I18N */ if (naccepted || check_node_accept (mctx, dfa->nodes + cur_node, str_idx)) { ok = re_node_set_insert (next_nodes, dfa->nexts[cur_node]); if (BE (! ok, 0)) { re_node_set_free (&union_set); return REG_ESPACE; } } } re_node_set_free (&union_set); return REG_NOERROR; } /* For all the nodes in CUR_NODES, add the epsilon closures of them to CUR_NODES, however exclude the nodes which are: - inside the sub expression whose number is EX_SUBEXP, if FL_OPEN. - out of the sub expression whose number is EX_SUBEXP, if !FL_OPEN. */ static reg_errcode_t check_arrival_expand_ecl (const re_dfa_t *dfa, re_node_set *cur_nodes, Idx ex_subexp, int type) { reg_errcode_t err; Idx idx, outside_node; re_node_set new_nodes; #ifdef DEBUG assert (cur_nodes->nelem); #endif err = re_node_set_alloc (&new_nodes, cur_nodes->nelem); if (BE (err != REG_NOERROR, 0)) return err; /* Create a new node set NEW_NODES with the nodes which are epsilon closures of the node in CUR_NODES. */ for (idx = 0; idx < cur_nodes->nelem; ++idx) { Idx cur_node = cur_nodes->elems[idx]; const re_node_set *eclosure = dfa->eclosures + cur_node; outside_node = find_subexp_node (dfa, eclosure, ex_subexp, type); if (outside_node == -1) { /* There are no problematic nodes, just merge them. */ err = re_node_set_merge (&new_nodes, eclosure); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&new_nodes); return err; } } else { /* There are problematic nodes, re-calculate incrementally. */ err = check_arrival_expand_ecl_sub (dfa, &new_nodes, cur_node, ex_subexp, type); if (BE (err != REG_NOERROR, 0)) { re_node_set_free (&new_nodes); return err; } } } re_node_set_free (cur_nodes); *cur_nodes = new_nodes; return REG_NOERROR; } /* Helper function for check_arrival_expand_ecl. Check incrementally the epsilon closure of TARGET, and if it isn't problematic append it to DST_NODES. */ static reg_errcode_t __attribute_warn_unused_result__ check_arrival_expand_ecl_sub (const re_dfa_t *dfa, re_node_set *dst_nodes, Idx target, Idx ex_subexp, int type) { Idx cur_node; for (cur_node = target; !re_node_set_contains (dst_nodes, cur_node);) { bool ok; if (dfa->nodes[cur_node].type == type && dfa->nodes[cur_node].opr.idx == ex_subexp) { if (type == OP_CLOSE_SUBEXP) { ok = re_node_set_insert (dst_nodes, cur_node); if (BE (! ok, 0)) return REG_ESPACE; } break; } ok = re_node_set_insert (dst_nodes, cur_node); if (BE (! ok, 0)) return REG_ESPACE; if (dfa->edests[cur_node].nelem == 0) break; if (dfa->edests[cur_node].nelem == 2) { reg_errcode_t err; err = check_arrival_expand_ecl_sub (dfa, dst_nodes, dfa->edests[cur_node].elems[1], ex_subexp, type); if (BE (err != REG_NOERROR, 0)) return err; } cur_node = dfa->edests[cur_node].elems[0]; } return REG_NOERROR; } /* For all the back references in the current state, calculate the destination of the back references by the appropriate entry in MCTX->BKREF_ENTS. */ static reg_errcode_t __attribute_warn_unused_result__ expand_bkref_cache (re_match_context_t *mctx, re_node_set *cur_nodes, Idx cur_str, Idx subexp_num, int type) { const re_dfa_t *const dfa = mctx->dfa; reg_errcode_t err; Idx cache_idx_start = search_cur_bkref_entry (mctx, cur_str); struct re_backref_cache_entry *ent; if (cache_idx_start == -1) return REG_NOERROR; restart: ent = mctx->bkref_ents + cache_idx_start; do { Idx to_idx, next_node; /* Is this entry ENT is appropriate? */ if (!re_node_set_contains (cur_nodes, ent->node)) continue; /* No. */ to_idx = cur_str + ent->subexp_to - ent->subexp_from; /* Calculate the destination of the back reference, and append it to MCTX->STATE_LOG. */ if (to_idx == cur_str) { /* The backreference did epsilon transit, we must re-check all the node in the current state. */ re_node_set new_dests; reg_errcode_t err2, err3; next_node = dfa->edests[ent->node].elems[0]; if (re_node_set_contains (cur_nodes, next_node)) continue; err = re_node_set_init_1 (&new_dests, next_node); err2 = check_arrival_expand_ecl (dfa, &new_dests, subexp_num, type); err3 = re_node_set_merge (cur_nodes, &new_dests); re_node_set_free (&new_dests); if (BE (err != REG_NOERROR || err2 != REG_NOERROR || err3 != REG_NOERROR, 0)) { err = (err != REG_NOERROR ? err : (err2 != REG_NOERROR ? err2 : err3)); return err; } /* TODO: It is still inefficient... */ goto restart; } else { re_node_set union_set; next_node = dfa->nexts[ent->node]; if (mctx->state_log[to_idx]) { bool ok; if (re_node_set_contains (&mctx->state_log[to_idx]->nodes, next_node)) continue; err = re_node_set_init_copy (&union_set, &mctx->state_log[to_idx]->nodes); ok = re_node_set_insert (&union_set, next_node); if (BE (err != REG_NOERROR || ! ok, 0)) { re_node_set_free (&union_set); err = err != REG_NOERROR ? err : REG_ESPACE; return err; } } else { err = re_node_set_init_1 (&union_set, next_node); if (BE (err != REG_NOERROR, 0)) return err; } mctx->state_log[to_idx] = re_acquire_state (&err, dfa, &union_set); re_node_set_free (&union_set); if (BE (mctx->state_log[to_idx] == NULL && err != REG_NOERROR, 0)) return err; } } while (ent++->more); return REG_NOERROR; } /* Build transition table for the state. Return true if successful. */ static bool build_trtable (const re_dfa_t *dfa, re_dfastate_t *state) { reg_errcode_t err; Idx i, j; int ch; bool need_word_trtable = false; bitset_word_t elem, mask; bool dests_node_malloced = false; bool dest_states_malloced = false; Idx ndests; /* Number of the destination states from 'state'. */ re_dfastate_t **trtable; re_dfastate_t **dest_states = NULL, **dest_states_word, **dest_states_nl; re_node_set follows, *dests_node; bitset_t *dests_ch; bitset_t acceptable; struct dests_alloc { re_node_set dests_node[SBC_MAX]; bitset_t dests_ch[SBC_MAX]; } *dests_alloc; /* We build DFA states which corresponds to the destination nodes from 'state'. 'dests_node[i]' represents the nodes which i-th destination state contains, and 'dests_ch[i]' represents the characters which i-th destination state accepts. */ if (__libc_use_alloca (sizeof (struct dests_alloc))) dests_alloc = (struct dests_alloc *) alloca (sizeof (struct dests_alloc)); else { dests_alloc = re_malloc (struct dests_alloc, 1); if (BE (dests_alloc == NULL, 0)) return false; dests_node_malloced = true; } dests_node = dests_alloc->dests_node; dests_ch = dests_alloc->dests_ch; /* Initialize transition table. */ state->word_trtable = state->trtable = NULL; /* At first, group all nodes belonging to 'state' into several destinations. */ ndests = group_nodes_into_DFAstates (dfa, state, dests_node, dests_ch); if (BE (ndests <= 0, 0)) { if (dests_node_malloced) re_free (dests_alloc); /* Return false in case of an error, true otherwise. */ if (ndests == 0) { state->trtable = (re_dfastate_t **) calloc (sizeof (re_dfastate_t *), SBC_MAX); if (BE (state->trtable == NULL, 0)) return false; return true; } return false; } err = re_node_set_alloc (&follows, ndests + 1); if (BE (err != REG_NOERROR, 0)) goto out_free; /* Avoid arithmetic overflow in size calculation. */ if (BE ((((SIZE_MAX - (sizeof (re_node_set) + sizeof (bitset_t)) * SBC_MAX) / (3 * sizeof (re_dfastate_t *))) < ndests), 0)) goto out_free; if (__libc_use_alloca ((sizeof (re_node_set) + sizeof (bitset_t)) * SBC_MAX + ndests * 3 * sizeof (re_dfastate_t *))) dest_states = (re_dfastate_t **) alloca (ndests * 3 * sizeof (re_dfastate_t *)); else { dest_states = re_malloc (re_dfastate_t *, ndests * 3); if (BE (dest_states == NULL, 0)) { out_free: if (dest_states_malloced) re_free (dest_states); re_node_set_free (&follows); for (i = 0; i < ndests; ++i) re_node_set_free (dests_node + i); if (dests_node_malloced) re_free (dests_alloc); return false; } dest_states_malloced = true; } dest_states_word = dest_states + ndests; dest_states_nl = dest_states_word + ndests; bitset_empty (acceptable); /* Then build the states for all destinations. */ for (i = 0; i < ndests; ++i) { Idx next_node; re_node_set_empty (&follows); /* Merge the follows of this destination states. */ for (j = 0; j < dests_node[i].nelem; ++j) { next_node = dfa->nexts[dests_node[i].elems[j]]; if (next_node != -1) { err = re_node_set_merge (&follows, dfa->eclosures + next_node); if (BE (err != REG_NOERROR, 0)) goto out_free; } } dest_states[i] = re_acquire_state_context (&err, dfa, &follows, 0); if (BE (dest_states[i] == NULL && err != REG_NOERROR, 0)) goto out_free; /* If the new state has context constraint, build appropriate states for these contexts. */ if (dest_states[i]->has_constraint) { dest_states_word[i] = re_acquire_state_context (&err, dfa, &follows, CONTEXT_WORD); if (BE (dest_states_word[i] == NULL && err != REG_NOERROR, 0)) goto out_free; if (dest_states[i] != dest_states_word[i] && dfa->mb_cur_max > 1) need_word_trtable = true; dest_states_nl[i] = re_acquire_state_context (&err, dfa, &follows, CONTEXT_NEWLINE); if (BE (dest_states_nl[i] == NULL && err != REG_NOERROR, 0)) goto out_free; } else { dest_states_word[i] = dest_states[i]; dest_states_nl[i] = dest_states[i]; } bitset_merge (acceptable, dests_ch[i]); } if (!BE (need_word_trtable, 0)) { /* We don't care about whether the following character is a word character, or we are in a single-byte character set so we can discern by looking at the character code: allocate a 256-entry transition table. */ trtable = state->trtable = (re_dfastate_t **) calloc (sizeof (re_dfastate_t *), SBC_MAX); if (BE (trtable == NULL, 0)) goto out_free; /* For all characters ch...: */ for (i = 0; i < BITSET_WORDS; ++i) for (ch = i * BITSET_WORD_BITS, elem = acceptable[i], mask = 1; elem; mask <<= 1, elem >>= 1, ++ch) if (BE (elem & 1, 0)) { /* There must be exactly one destination which accepts character ch. See group_nodes_into_DFAstates. */ for (j = 0; (dests_ch[j][i] & mask) == 0; ++j) ; /* j-th destination accepts the word character ch. */ if (dfa->word_char[i] & mask) trtable[ch] = dest_states_word[j]; else trtable[ch] = dest_states[j]; } } else { /* We care about whether the following character is a word character, and we are in a multi-byte character set: discern by looking at the character code: build two 256-entry transition tables, one starting at trtable[0] and one starting at trtable[SBC_MAX]. */ trtable = state->word_trtable = (re_dfastate_t **) calloc (sizeof (re_dfastate_t *), 2 * SBC_MAX); if (BE (trtable == NULL, 0)) goto out_free; /* For all characters ch...: */ for (i = 0; i < BITSET_WORDS; ++i) for (ch = i * BITSET_WORD_BITS, elem = acceptable[i], mask = 1; elem; mask <<= 1, elem >>= 1, ++ch) if (BE (elem & 1, 0)) { /* There must be exactly one destination which accepts character ch. See group_nodes_into_DFAstates. */ for (j = 0; (dests_ch[j][i] & mask) == 0; ++j) ; /* j-th destination accepts the word character ch. */ trtable[ch] = dest_states[j]; trtable[ch + SBC_MAX] = dest_states_word[j]; } } /* new line */ if (bitset_contain (acceptable, NEWLINE_CHAR)) { /* The current state accepts newline character. */ for (j = 0; j < ndests; ++j) if (bitset_contain (dests_ch[j], NEWLINE_CHAR)) { /* k-th destination accepts newline character. */ trtable[NEWLINE_CHAR] = dest_states_nl[j]; if (need_word_trtable) trtable[NEWLINE_CHAR + SBC_MAX] = dest_states_nl[j]; /* There must be only one destination which accepts newline. See group_nodes_into_DFAstates. */ break; } } if (dest_states_malloced) re_free (dest_states); re_node_set_free (&follows); for (i = 0; i < ndests; ++i) re_node_set_free (dests_node + i); if (dests_node_malloced) re_free (dests_alloc); return true; } /* Group all nodes belonging to STATE into several destinations. Then for all destinations, set the nodes belonging to the destination to DESTS_NODE[i] and set the characters accepted by the destination to DEST_CH[i]. This function return the number of destinations. */ static Idx group_nodes_into_DFAstates (const re_dfa_t *dfa, const re_dfastate_t *state, re_node_set *dests_node, bitset_t *dests_ch) { reg_errcode_t err; bool ok; Idx i, j, k; Idx ndests; /* Number of the destinations from 'state'. */ bitset_t accepts; /* Characters a node can accept. */ const re_node_set *cur_nodes = &state->nodes; bitset_empty (accepts); ndests = 0; /* For all the nodes belonging to 'state', */ for (i = 0; i < cur_nodes->nelem; ++i) { re_token_t *node = &dfa->nodes[cur_nodes->elems[i]]; re_token_type_t type = node->type; unsigned int constraint = node->constraint; /* Enumerate all single byte character this node can accept. */ if (type == CHARACTER) bitset_set (accepts, node->opr.c); else if (type == SIMPLE_BRACKET) { bitset_merge (accepts, node->opr.sbcset); } else if (type == OP_PERIOD) { #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) bitset_merge (accepts, dfa->sb_char); else #endif bitset_set_all (accepts); if (!(dfa->syntax & RE_DOT_NEWLINE)) bitset_clear (accepts, '\n'); if (dfa->syntax & RE_DOT_NOT_NULL) bitset_clear (accepts, '\0'); } #ifdef RE_ENABLE_I18N else if (type == OP_UTF8_PERIOD) { if (ASCII_CHARS % BITSET_WORD_BITS == 0) memset (accepts, -1, ASCII_CHARS / CHAR_BIT); else bitset_merge (accepts, utf8_sb_map); if (!(dfa->syntax & RE_DOT_NEWLINE)) bitset_clear (accepts, '\n'); if (dfa->syntax & RE_DOT_NOT_NULL) bitset_clear (accepts, '\0'); } #endif else continue; /* Check the 'accepts' and sift the characters which are not match it the context. */ if (constraint) { if (constraint & NEXT_NEWLINE_CONSTRAINT) { bool accepts_newline = bitset_contain (accepts, NEWLINE_CHAR); bitset_empty (accepts); if (accepts_newline) bitset_set (accepts, NEWLINE_CHAR); else continue; } if (constraint & NEXT_ENDBUF_CONSTRAINT) { bitset_empty (accepts); continue; } if (constraint & NEXT_WORD_CONSTRAINT) { bitset_word_t any_set = 0; if (type == CHARACTER && !node->word_char) { bitset_empty (accepts); continue; } #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= (dfa->word_char[j] | ~dfa->sb_char[j])); else #endif for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= dfa->word_char[j]); if (!any_set) continue; } if (constraint & NEXT_NOTWORD_CONSTRAINT) { bitset_word_t any_set = 0; if (type == CHARACTER && node->word_char) { bitset_empty (accepts); continue; } #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= ~(dfa->word_char[j] & dfa->sb_char[j])); else #endif for (j = 0; j < BITSET_WORDS; ++j) any_set |= (accepts[j] &= ~dfa->word_char[j]); if (!any_set) continue; } } /* Then divide 'accepts' into DFA states, or create a new state. Above, we make sure that accepts is not empty. */ for (j = 0; j < ndests; ++j) { bitset_t intersec; /* Intersection sets, see below. */ bitset_t remains; /* Flags, see below. */ bitset_word_t has_intersec, not_subset, not_consumed; /* Optimization, skip if this state doesn't accept the character. */ if (type == CHARACTER && !bitset_contain (dests_ch[j], node->opr.c)) continue; /* Enumerate the intersection set of this state and 'accepts'. */ has_intersec = 0; for (k = 0; k < BITSET_WORDS; ++k) has_intersec |= intersec[k] = accepts[k] & dests_ch[j][k]; /* And skip if the intersection set is empty. */ if (!has_intersec) continue; /* Then check if this state is a subset of 'accepts'. */ not_subset = not_consumed = 0; for (k = 0; k < BITSET_WORDS; ++k) { not_subset |= remains[k] = ~accepts[k] & dests_ch[j][k]; not_consumed |= accepts[k] = accepts[k] & ~dests_ch[j][k]; } /* If this state isn't a subset of 'accepts', create a new group state, which has the 'remains'. */ if (not_subset) { bitset_copy (dests_ch[ndests], remains); bitset_copy (dests_ch[j], intersec); err = re_node_set_init_copy (dests_node + ndests, &dests_node[j]); if (BE (err != REG_NOERROR, 0)) goto error_return; ++ndests; } /* Put the position in the current group. */ ok = re_node_set_insert (&dests_node[j], cur_nodes->elems[i]); if (BE (! ok, 0)) goto error_return; /* If all characters are consumed, go to next node. */ if (!not_consumed) break; } /* Some characters remain, create a new group. */ if (j == ndests) { bitset_copy (dests_ch[ndests], accepts); err = re_node_set_init_1 (dests_node + ndests, cur_nodes->elems[i]); if (BE (err != REG_NOERROR, 0)) goto error_return; ++ndests; bitset_empty (accepts); } } return ndests; error_return: for (j = 0; j < ndests; ++j) re_node_set_free (dests_node + j); return -1; } #ifdef RE_ENABLE_I18N /* Check how many bytes the node 'dfa->nodes[node_idx]' accepts. Return the number of the bytes the node accepts. STR_IDX is the current index of the input string. This function handles the nodes which can accept one character, or one collating element like '.', '[a-z]', opposite to the other nodes can only accept one byte. */ # ifdef _LIBC # include # endif static int check_node_accept_bytes (const re_dfa_t *dfa, Idx node_idx, const re_string_t *input, Idx str_idx) { const re_token_t *node = dfa->nodes + node_idx; int char_len, elem_len; Idx i; if (BE (node->type == OP_UTF8_PERIOD, 0)) { unsigned char c = re_string_byte_at (input, str_idx), d; if (BE (c < 0xc2, 1)) return 0; if (str_idx + 2 > input->len) return 0; d = re_string_byte_at (input, str_idx + 1); if (c < 0xe0) return (d < 0x80 || d > 0xbf) ? 0 : 2; else if (c < 0xf0) { char_len = 3; if (c == 0xe0 && d < 0xa0) return 0; } else if (c < 0xf8) { char_len = 4; if (c == 0xf0 && d < 0x90) return 0; } else if (c < 0xfc) { char_len = 5; if (c == 0xf8 && d < 0x88) return 0; } else if (c < 0xfe) { char_len = 6; if (c == 0xfc && d < 0x84) return 0; } else return 0; if (str_idx + char_len > input->len) return 0; for (i = 1; i < char_len; ++i) { d = re_string_byte_at (input, str_idx + i); if (d < 0x80 || d > 0xbf) return 0; } return char_len; } char_len = re_string_char_size_at (input, str_idx); if (node->type == OP_PERIOD) { if (char_len <= 1) return 0; /* FIXME: I don't think this if is needed, as both '\n' and '\0' are char_len == 1. */ /* '.' accepts any one character except the following two cases. */ if ((!(dfa->syntax & RE_DOT_NEWLINE) && re_string_byte_at (input, str_idx) == '\n') || ((dfa->syntax & RE_DOT_NOT_NULL) && re_string_byte_at (input, str_idx) == '\0')) return 0; return char_len; } elem_len = re_string_elem_size_at (input, str_idx); if ((elem_len <= 1 && char_len <= 1) || char_len == 0) return 0; if (node->type == COMPLEX_BRACKET) { const re_charset_t *cset = node->opr.mbcset; # ifdef _LIBC const unsigned char *pin = ((const unsigned char *) re_string_get_buffer (input) + str_idx); Idx j; uint32_t nrules; # endif /* _LIBC */ int match_len = 0; wchar_t wc = ((cset->nranges || cset->nchar_classes || cset->nmbchars) ? re_string_wchar_at (input, str_idx) : 0); /* match with multibyte character? */ for (i = 0; i < cset->nmbchars; ++i) if (wc == cset->mbchars[i]) { match_len = char_len; goto check_node_accept_bytes_match; } /* match with character_class? */ for (i = 0; i < cset->nchar_classes; ++i) { wctype_t wt = cset->char_classes[i]; if (__iswctype (wc, wt)) { match_len = char_len; goto check_node_accept_bytes_match; } } # ifdef _LIBC nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules != 0) { unsigned int in_collseq = 0; const int32_t *table, *indirect; const unsigned char *weights, *extra; const char *collseqwc; /* match with collating_symbol? */ if (cset->ncoll_syms) extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB); for (i = 0; i < cset->ncoll_syms; ++i) { const unsigned char *coll_sym = extra + cset->coll_syms[i]; /* Compare the length of input collating element and the length of current collating element. */ if (*coll_sym != elem_len) continue; /* Compare each bytes. */ for (j = 0; j < *coll_sym; j++) if (pin[j] != coll_sym[1 + j]) break; if (j == *coll_sym) { /* Match if every bytes is equal. */ match_len = j; goto check_node_accept_bytes_match; } } if (cset->nranges) { if (elem_len <= char_len) { collseqwc = _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQWC); in_collseq = __collseq_table_lookup (collseqwc, wc); } else in_collseq = find_collation_sequence_value (pin, elem_len); } /* match with range expression? */ /* FIXME: Implement rational ranges here, too. */ for (i = 0; i < cset->nranges; ++i) if (cset->range_starts[i] <= in_collseq && in_collseq <= cset->range_ends[i]) { match_len = elem_len; goto check_node_accept_bytes_match; } /* match with equivalence_class? */ if (cset->nequiv_classes) { const unsigned char *cp = pin; table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); weights = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_WEIGHTMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_EXTRAMB); indirect = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_INDIRECTMB); int32_t idx = findidx (table, indirect, extra, &cp, elem_len); if (idx > 0) for (i = 0; i < cset->nequiv_classes; ++i) { int32_t equiv_class_idx = cset->equiv_classes[i]; size_t weight_len = weights[idx & 0xffffff]; if (weight_len == weights[equiv_class_idx & 0xffffff] && (idx >> 24) == (equiv_class_idx >> 24)) { Idx cnt = 0; idx &= 0xffffff; equiv_class_idx &= 0xffffff; while (cnt <= weight_len && (weights[equiv_class_idx + 1 + cnt] == weights[idx + 1 + cnt])) ++cnt; if (cnt > weight_len) { match_len = elem_len; goto check_node_accept_bytes_match; } } } } } else # endif /* _LIBC */ { /* match with range expression? */ for (i = 0; i < cset->nranges; ++i) { if (cset->range_starts[i] <= wc && wc <= cset->range_ends[i]) { match_len = char_len; goto check_node_accept_bytes_match; } } } check_node_accept_bytes_match: if (!cset->non_match) return match_len; else { if (match_len > 0) return 0; else return (elem_len > char_len) ? elem_len : char_len; } } return 0; } # ifdef _LIBC static unsigned int find_collation_sequence_value (const unsigned char *mbs, size_t mbs_len) { uint32_t nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules == 0) { if (mbs_len == 1) { /* No valid character. Match it as a single byte character. */ const unsigned char *collseq = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQMB); return collseq[mbs[0]]; } return UINT_MAX; } else { int32_t idx; const unsigned char *extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB); int32_t extrasize = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB + 1) - extra; for (idx = 0; idx < extrasize;) { int mbs_cnt; bool found = false; int32_t elem_mbs_len; /* Skip the name of collating element name. */ idx = idx + extra[idx] + 1; elem_mbs_len = extra[idx++]; if (mbs_len == elem_mbs_len) { for (mbs_cnt = 0; mbs_cnt < elem_mbs_len; ++mbs_cnt) if (extra[idx + mbs_cnt] != mbs[mbs_cnt]) break; if (mbs_cnt == elem_mbs_len) /* Found the entry. */ found = true; } /* Skip the byte sequence of the collating element. */ idx += elem_mbs_len; /* Adjust for the alignment. */ idx = (idx + 3) & ~3; /* Skip the collation sequence value. */ idx += sizeof (uint32_t); /* Skip the wide char sequence of the collating element. */ idx = idx + sizeof (uint32_t) * (*(int32_t *) (extra + idx) + 1); /* If we found the entry, return the sequence value. */ if (found) return *(uint32_t *) (extra + idx); /* Skip the collation sequence value. */ idx += sizeof (uint32_t); } return UINT_MAX; } } # endif /* _LIBC */ #endif /* RE_ENABLE_I18N */ /* Check whether the node accepts the byte which is IDX-th byte of the INPUT. */ static bool check_node_accept (const re_match_context_t *mctx, const re_token_t *node, Idx idx) { unsigned char ch; ch = re_string_byte_at (&mctx->input, idx); switch (node->type) { case CHARACTER: if (node->opr.c != ch) return false; break; case SIMPLE_BRACKET: if (!bitset_contain (node->opr.sbcset, ch)) return false; break; #ifdef RE_ENABLE_I18N case OP_UTF8_PERIOD: if (ch >= ASCII_CHARS) return false; FALLTHROUGH; #endif case OP_PERIOD: if ((ch == '\n' && !(mctx->dfa->syntax & RE_DOT_NEWLINE)) || (ch == '\0' && (mctx->dfa->syntax & RE_DOT_NOT_NULL))) return false; break; default: return false; } if (node->constraint) { /* The node has constraints. Check whether the current context satisfies the constraints. */ unsigned int context = re_string_context_at (&mctx->input, idx, mctx->eflags); if (NOT_SATISFY_NEXT_CONSTRAINT (node->constraint, context)) return false; } return true; } /* Extend the buffers, if the buffers have run out. */ static reg_errcode_t __attribute_warn_unused_result__ extend_buffers (re_match_context_t *mctx, int min_len) { reg_errcode_t ret; re_string_t *pstr = &mctx->input; /* Avoid overflow. */ if (BE (MIN (IDX_MAX, SIZE_MAX / sizeof (re_dfastate_t *)) / 2 <= pstr->bufs_len, 0)) return REG_ESPACE; /* Double the lengths of the buffers, but allocate at least MIN_LEN. */ ret = re_string_realloc_buffers (pstr, MAX (min_len, MIN (pstr->len, pstr->bufs_len * 2))); if (BE (ret != REG_NOERROR, 0)) return ret; if (mctx->state_log != NULL) { /* And double the length of state_log. */ /* XXX We have no indication of the size of this buffer. If this allocation fail we have no indication that the state_log array does not have the right size. */ re_dfastate_t **new_array = re_realloc (mctx->state_log, re_dfastate_t *, pstr->bufs_len + 1); if (BE (new_array == NULL, 0)) return REG_ESPACE; mctx->state_log = new_array; } /* Then reconstruct the buffers. */ if (pstr->icase) { #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { ret = build_wcs_upper_buffer (pstr); if (BE (ret != REG_NOERROR, 0)) return ret; } else #endif /* RE_ENABLE_I18N */ build_upper_buffer (pstr); } else { #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) build_wcs_buffer (pstr); else #endif /* RE_ENABLE_I18N */ { if (pstr->trans != NULL) re_string_translate_buffer (pstr); } } return REG_NOERROR; } /* Functions for matching context. */ /* Initialize MCTX. */ static reg_errcode_t __attribute_warn_unused_result__ match_ctx_init (re_match_context_t *mctx, int eflags, Idx n) { mctx->eflags = eflags; mctx->match_last = -1; if (n > 0) { /* Avoid overflow. */ size_t max_object_size = MAX (sizeof (struct re_backref_cache_entry), sizeof (re_sub_match_top_t *)); if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) < n, 0)) return REG_ESPACE; mctx->bkref_ents = re_malloc (struct re_backref_cache_entry, n); mctx->sub_tops = re_malloc (re_sub_match_top_t *, n); if (BE (mctx->bkref_ents == NULL || mctx->sub_tops == NULL, 0)) return REG_ESPACE; } /* Already zero-ed by the caller. else mctx->bkref_ents = NULL; mctx->nbkref_ents = 0; mctx->nsub_tops = 0; */ mctx->abkref_ents = n; mctx->max_mb_elem_len = 1; mctx->asub_tops = n; return REG_NOERROR; } /* Clean the entries which depend on the current input in MCTX. This function must be invoked when the matcher changes the start index of the input, or changes the input string. */ static void match_ctx_clean (re_match_context_t *mctx) { Idx st_idx; for (st_idx = 0; st_idx < mctx->nsub_tops; ++st_idx) { Idx sl_idx; re_sub_match_top_t *top = mctx->sub_tops[st_idx]; for (sl_idx = 0; sl_idx < top->nlasts; ++sl_idx) { re_sub_match_last_t *last = top->lasts[sl_idx]; re_free (last->path.array); re_free (last); } re_free (top->lasts); if (top->path) { re_free (top->path->array); re_free (top->path); } re_free (top); } mctx->nsub_tops = 0; mctx->nbkref_ents = 0; } /* Free all the memory associated with MCTX. */ static void match_ctx_free (re_match_context_t *mctx) { /* First, free all the memory associated with MCTX->SUB_TOPS. */ match_ctx_clean (mctx); re_free (mctx->sub_tops); re_free (mctx->bkref_ents); } /* Add a new backreference entry to MCTX. Note that we assume that caller never call this function with duplicate entry, and call with STR_IDX which isn't smaller than any existing entry. */ static reg_errcode_t __attribute_warn_unused_result__ match_ctx_add_entry (re_match_context_t *mctx, Idx node, Idx str_idx, Idx from, Idx to) { if (mctx->nbkref_ents >= mctx->abkref_ents) { struct re_backref_cache_entry* new_entry; new_entry = re_realloc (mctx->bkref_ents, struct re_backref_cache_entry, mctx->abkref_ents * 2); if (BE (new_entry == NULL, 0)) { re_free (mctx->bkref_ents); return REG_ESPACE; } mctx->bkref_ents = new_entry; memset (mctx->bkref_ents + mctx->nbkref_ents, '\0', sizeof (struct re_backref_cache_entry) * mctx->abkref_ents); mctx->abkref_ents *= 2; } if (mctx->nbkref_ents > 0 && mctx->bkref_ents[mctx->nbkref_ents - 1].str_idx == str_idx) mctx->bkref_ents[mctx->nbkref_ents - 1].more = 1; mctx->bkref_ents[mctx->nbkref_ents].node = node; mctx->bkref_ents[mctx->nbkref_ents].str_idx = str_idx; mctx->bkref_ents[mctx->nbkref_ents].subexp_from = from; mctx->bkref_ents[mctx->nbkref_ents].subexp_to = to; /* This is a cache that saves negative results of check_dst_limits_calc_pos. If bit N is clear, means that this entry won't epsilon-transition to an OP_OPEN_SUBEXP or OP_CLOSE_SUBEXP for the N+1-th subexpression. If it is set, check_dst_limits_calc_pos_1 will recurse and try to find one such node. A backreference does not epsilon-transition unless it is empty, so set to all zeros if FROM != TO. */ mctx->bkref_ents[mctx->nbkref_ents].eps_reachable_subexps_map = (from == to ? -1 : 0); mctx->bkref_ents[mctx->nbkref_ents++].more = 0; if (mctx->max_mb_elem_len < to - from) mctx->max_mb_elem_len = to - from; return REG_NOERROR; } /* Return the first entry with the same str_idx, or -1 if none is found. Note that MCTX->BKREF_ENTS is already sorted by MCTX->STR_IDX. */ static Idx search_cur_bkref_entry (const re_match_context_t *mctx, Idx str_idx) { Idx left, right, mid, last; last = right = mctx->nbkref_ents; for (left = 0; left < right;) { mid = (left + right) / 2; if (mctx->bkref_ents[mid].str_idx < str_idx) left = mid + 1; else right = mid; } if (left < last && mctx->bkref_ents[left].str_idx == str_idx) return left; else return -1; } /* Register the node NODE, whose type is OP_OPEN_SUBEXP, and which matches at STR_IDX. */ static reg_errcode_t __attribute_warn_unused_result__ match_ctx_add_subtop (re_match_context_t *mctx, Idx node, Idx str_idx) { #ifdef DEBUG assert (mctx->sub_tops != NULL); assert (mctx->asub_tops > 0); #endif if (BE (mctx->nsub_tops == mctx->asub_tops, 0)) { Idx new_asub_tops = mctx->asub_tops * 2; re_sub_match_top_t **new_array = re_realloc (mctx->sub_tops, re_sub_match_top_t *, new_asub_tops); if (BE (new_array == NULL, 0)) return REG_ESPACE; mctx->sub_tops = new_array; mctx->asub_tops = new_asub_tops; } mctx->sub_tops[mctx->nsub_tops] = calloc (1, sizeof (re_sub_match_top_t)); if (BE (mctx->sub_tops[mctx->nsub_tops] == NULL, 0)) return REG_ESPACE; mctx->sub_tops[mctx->nsub_tops]->node = node; mctx->sub_tops[mctx->nsub_tops++]->str_idx = str_idx; return REG_NOERROR; } /* Register the node NODE, whose type is OP_CLOSE_SUBEXP, and which matches at STR_IDX, whose corresponding OP_OPEN_SUBEXP is SUB_TOP. */ static re_sub_match_last_t * match_ctx_add_sublast (re_sub_match_top_t *subtop, Idx node, Idx str_idx) { re_sub_match_last_t *new_entry; if (BE (subtop->nlasts == subtop->alasts, 0)) { Idx new_alasts = 2 * subtop->alasts + 1; re_sub_match_last_t **new_array = re_realloc (subtop->lasts, re_sub_match_last_t *, new_alasts); if (BE (new_array == NULL, 0)) return NULL; subtop->lasts = new_array; subtop->alasts = new_alasts; } new_entry = calloc (1, sizeof (re_sub_match_last_t)); if (BE (new_entry != NULL, 1)) { subtop->lasts[subtop->nlasts] = new_entry; new_entry->node = node; new_entry->str_idx = str_idx; ++subtop->nlasts; } return new_entry; } static void sift_ctx_init (re_sift_context_t *sctx, re_dfastate_t **sifted_sts, re_dfastate_t **limited_sts, Idx last_node, Idx last_str_idx) { sctx->sifted_states = sifted_sts; sctx->limited_states = limited_sts; sctx->last_node = last_node; sctx->last_str_idx = last_str_idx; re_node_set_init_empty (&sctx->limits); } gnuastro-0.5/bootstrapped/lib/regex_internal.c0000644000175000017500000013532413217200021016563 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ static void re_string_construct_common (const char *str, Idx len, re_string_t *pstr, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa); static re_dfastate_t *create_ci_newstate (const re_dfa_t *dfa, const re_node_set *nodes, re_hashval_t hash); static re_dfastate_t *create_cd_newstate (const re_dfa_t *dfa, const re_node_set *nodes, unsigned int context, re_hashval_t hash); /* Functions for string operation. */ /* This function allocate the buffers. It is necessary to call re_string_reconstruct before using the object. */ static reg_errcode_t __attribute_warn_unused_result__ re_string_allocate (re_string_t *pstr, const char *str, Idx len, Idx init_len, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) { reg_errcode_t ret; Idx init_buf_len; /* Ensure at least one character fits into the buffers. */ if (init_len < dfa->mb_cur_max) init_len = dfa->mb_cur_max; init_buf_len = (len + 1 < init_len) ? len + 1: init_len; re_string_construct_common (str, len, pstr, trans, icase, dfa); ret = re_string_realloc_buffers (pstr, init_buf_len); if (BE (ret != REG_NOERROR, 0)) return ret; pstr->word_char = dfa->word_char; pstr->word_ops_used = dfa->word_ops_used; pstr->mbs = pstr->mbs_allocated ? pstr->mbs : (unsigned char *) str; pstr->valid_len = (pstr->mbs_allocated || dfa->mb_cur_max > 1) ? 0 : len; pstr->valid_raw_len = pstr->valid_len; return REG_NOERROR; } /* This function allocate the buffers, and initialize them. */ static reg_errcode_t __attribute_warn_unused_result__ re_string_construct (re_string_t *pstr, const char *str, Idx len, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) { reg_errcode_t ret; memset (pstr, '\0', sizeof (re_string_t)); re_string_construct_common (str, len, pstr, trans, icase, dfa); if (len > 0) { ret = re_string_realloc_buffers (pstr, len + 1); if (BE (ret != REG_NOERROR, 0)) return ret; } pstr->mbs = pstr->mbs_allocated ? pstr->mbs : (unsigned char *) str; if (icase) { #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { while (1) { ret = build_wcs_upper_buffer (pstr); if (BE (ret != REG_NOERROR, 0)) return ret; if (pstr->valid_raw_len >= len) break; if (pstr->bufs_len > pstr->valid_len + dfa->mb_cur_max) break; ret = re_string_realloc_buffers (pstr, pstr->bufs_len * 2); if (BE (ret != REG_NOERROR, 0)) return ret; } } else #endif /* RE_ENABLE_I18N */ build_upper_buffer (pstr); } else { #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) build_wcs_buffer (pstr); else #endif /* RE_ENABLE_I18N */ { if (trans != NULL) re_string_translate_buffer (pstr); else { pstr->valid_len = pstr->bufs_len; pstr->valid_raw_len = pstr->bufs_len; } } } return REG_NOERROR; } /* Helper functions for re_string_allocate, and re_string_construct. */ static reg_errcode_t __attribute_warn_unused_result__ re_string_realloc_buffers (re_string_t *pstr, Idx new_buf_len) { #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { wint_t *new_wcs; /* Avoid overflow in realloc. */ const size_t max_object_size = MAX (sizeof (wint_t), sizeof (Idx)); if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) < new_buf_len, 0)) return REG_ESPACE; new_wcs = re_realloc (pstr->wcs, wint_t, new_buf_len); if (BE (new_wcs == NULL, 0)) return REG_ESPACE; pstr->wcs = new_wcs; if (pstr->offsets != NULL) { Idx *new_offsets = re_realloc (pstr->offsets, Idx, new_buf_len); if (BE (new_offsets == NULL, 0)) return REG_ESPACE; pstr->offsets = new_offsets; } } #endif /* RE_ENABLE_I18N */ if (pstr->mbs_allocated) { unsigned char *new_mbs = re_realloc (pstr->mbs, unsigned char, new_buf_len); if (BE (new_mbs == NULL, 0)) return REG_ESPACE; pstr->mbs = new_mbs; } pstr->bufs_len = new_buf_len; return REG_NOERROR; } static void re_string_construct_common (const char *str, Idx len, re_string_t *pstr, RE_TRANSLATE_TYPE trans, bool icase, const re_dfa_t *dfa) { pstr->raw_mbs = (const unsigned char *) str; pstr->len = len; pstr->raw_len = len; pstr->trans = trans; pstr->icase = icase; pstr->mbs_allocated = (trans != NULL || icase); pstr->mb_cur_max = dfa->mb_cur_max; pstr->is_utf8 = dfa->is_utf8; pstr->map_notascii = dfa->map_notascii; pstr->stop = pstr->len; pstr->raw_stop = pstr->stop; } #ifdef RE_ENABLE_I18N /* Build wide character buffer PSTR->WCS. If the byte sequence of the string are: (0), (1), (0), (1), Then wide character buffer will be: , WEOF , , WEOF , We use WEOF for padding, they indicate that the position isn't a first byte of a multibyte character. Note that this function assumes PSTR->VALID_LEN elements are already built and starts from PSTR->VALID_LEN. */ static void build_wcs_buffer (re_string_t *pstr) { #ifdef _LIBC unsigned char buf[MB_LEN_MAX]; assert (MB_LEN_MAX >= pstr->mb_cur_max); #else unsigned char buf[64]; #endif mbstate_t prev_st; Idx byte_idx, end_idx, remain_len; size_t mbclen; /* Build the buffers from pstr->valid_len to either pstr->len or pstr->bufs_len. */ end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; for (byte_idx = pstr->valid_len; byte_idx < end_idx;) { wchar_t wc; const char *p; remain_len = end_idx - byte_idx; prev_st = pstr->cur_state; /* Apply the translation if we need. */ if (BE (pstr->trans != NULL, 0)) { int i, ch; for (i = 0; i < pstr->mb_cur_max && i < remain_len; ++i) { ch = pstr->raw_mbs [pstr->raw_mbs_idx + byte_idx + i]; buf[i] = pstr->mbs[byte_idx + i] = pstr->trans[ch]; } p = (const char *) buf; } else p = (const char *) pstr->raw_mbs + pstr->raw_mbs_idx + byte_idx; mbclen = __mbrtowc (&wc, p, remain_len, &pstr->cur_state); if (BE (mbclen == (size_t) -1 || mbclen == 0 || (mbclen == (size_t) -2 && pstr->bufs_len >= pstr->len), 0)) { /* We treat these cases as a singlebyte character. */ mbclen = 1; wc = (wchar_t) pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]; if (BE (pstr->trans != NULL, 0)) wc = pstr->trans[wc]; pstr->cur_state = prev_st; } else if (BE (mbclen == (size_t) -2, 0)) { /* The buffer doesn't have enough space, finish to build. */ pstr->cur_state = prev_st; break; } /* Write wide character and padding. */ pstr->wcs[byte_idx++] = wc; /* Write paddings. */ for (remain_len = byte_idx + mbclen - 1; byte_idx < remain_len ;) pstr->wcs[byte_idx++] = WEOF; } pstr->valid_len = byte_idx; pstr->valid_raw_len = byte_idx; } /* Build wide character buffer PSTR->WCS like build_wcs_buffer, but for REG_ICASE. */ static reg_errcode_t __attribute_warn_unused_result__ build_wcs_upper_buffer (re_string_t *pstr) { mbstate_t prev_st; Idx src_idx, byte_idx, end_idx, remain_len; size_t mbclen; #ifdef _LIBC char buf[MB_LEN_MAX]; assert (MB_LEN_MAX >= pstr->mb_cur_max); #else char buf[64]; #endif byte_idx = pstr->valid_len; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; /* The following optimization assumes that ASCII characters can be mapped to wide characters with a simple cast. */ if (! pstr->map_notascii && pstr->trans == NULL && !pstr->offsets_needed) { while (byte_idx < end_idx) { wchar_t wc; if (isascii (pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]) && mbsinit (&pstr->cur_state)) { /* In case of a singlebyte character. */ pstr->mbs[byte_idx] = toupper (pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]); /* The next step uses the assumption that wchar_t is encoded ASCII-safe: all ASCII values can be converted like this. */ pstr->wcs[byte_idx] = (wchar_t) pstr->mbs[byte_idx]; ++byte_idx; continue; } remain_len = end_idx - byte_idx; prev_st = pstr->cur_state; mbclen = __mbrtowc (&wc, ((const char *) pstr->raw_mbs + pstr->raw_mbs_idx + byte_idx), remain_len, &pstr->cur_state); if (BE (mbclen < (size_t) -2, 1)) { wchar_t wcu = __towupper (wc); if (wcu != wc) { size_t mbcdlen; mbcdlen = __wcrtomb (buf, wcu, &prev_st); if (BE (mbclen == mbcdlen, 1)) memcpy (pstr->mbs + byte_idx, buf, mbclen); else { src_idx = byte_idx; goto offsets_needed; } } else memcpy (pstr->mbs + byte_idx, pstr->raw_mbs + pstr->raw_mbs_idx + byte_idx, mbclen); pstr->wcs[byte_idx++] = wcu; /* Write paddings. */ for (remain_len = byte_idx + mbclen - 1; byte_idx < remain_len ;) pstr->wcs[byte_idx++] = WEOF; } else if (mbclen == (size_t) -1 || mbclen == 0 || (mbclen == (size_t) -2 && pstr->bufs_len >= pstr->len)) { /* It is an invalid character, an incomplete character at the end of the string, or '\0'. Just use the byte. */ int ch = pstr->raw_mbs[pstr->raw_mbs_idx + byte_idx]; pstr->mbs[byte_idx] = ch; /* And also cast it to wide char. */ pstr->wcs[byte_idx++] = (wchar_t) ch; if (BE (mbclen == (size_t) -1, 0)) pstr->cur_state = prev_st; } else { /* The buffer doesn't have enough space, finish to build. */ pstr->cur_state = prev_st; break; } } pstr->valid_len = byte_idx; pstr->valid_raw_len = byte_idx; return REG_NOERROR; } else for (src_idx = pstr->valid_raw_len; byte_idx < end_idx;) { wchar_t wc; const char *p; offsets_needed: remain_len = end_idx - byte_idx; prev_st = pstr->cur_state; if (BE (pstr->trans != NULL, 0)) { int i, ch; for (i = 0; i < pstr->mb_cur_max && i < remain_len; ++i) { ch = pstr->raw_mbs [pstr->raw_mbs_idx + src_idx + i]; buf[i] = pstr->trans[ch]; } p = (const char *) buf; } else p = (const char *) pstr->raw_mbs + pstr->raw_mbs_idx + src_idx; mbclen = __mbrtowc (&wc, p, remain_len, &pstr->cur_state); if (BE (mbclen < (size_t) -2, 1)) { wchar_t wcu = __towupper (wc); if (wcu != wc) { size_t mbcdlen; mbcdlen = wcrtomb ((char *) buf, wcu, &prev_st); if (BE (mbclen == mbcdlen, 1)) memcpy (pstr->mbs + byte_idx, buf, mbclen); else if (mbcdlen != (size_t) -1) { size_t i; if (byte_idx + mbcdlen > pstr->bufs_len) { pstr->cur_state = prev_st; break; } if (pstr->offsets == NULL) { pstr->offsets = re_malloc (Idx, pstr->bufs_len); if (pstr->offsets == NULL) return REG_ESPACE; } if (!pstr->offsets_needed) { for (i = 0; i < (size_t) byte_idx; ++i) pstr->offsets[i] = i; pstr->offsets_needed = 1; } memcpy (pstr->mbs + byte_idx, buf, mbcdlen); pstr->wcs[byte_idx] = wcu; pstr->offsets[byte_idx] = src_idx; for (i = 1; i < mbcdlen; ++i) { pstr->offsets[byte_idx + i] = src_idx + (i < mbclen ? i : mbclen - 1); pstr->wcs[byte_idx + i] = WEOF; } pstr->len += mbcdlen - mbclen; if (pstr->raw_stop > src_idx) pstr->stop += mbcdlen - mbclen; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; byte_idx += mbcdlen; src_idx += mbclen; continue; } else memcpy (pstr->mbs + byte_idx, p, mbclen); } else memcpy (pstr->mbs + byte_idx, p, mbclen); if (BE (pstr->offsets_needed != 0, 0)) { size_t i; for (i = 0; i < mbclen; ++i) pstr->offsets[byte_idx + i] = src_idx + i; } src_idx += mbclen; pstr->wcs[byte_idx++] = wcu; /* Write paddings. */ for (remain_len = byte_idx + mbclen - 1; byte_idx < remain_len ;) pstr->wcs[byte_idx++] = WEOF; } else if (mbclen == (size_t) -1 || mbclen == 0 || (mbclen == (size_t) -2 && pstr->bufs_len >= pstr->len)) { /* It is an invalid character or '\0'. Just use the byte. */ int ch = pstr->raw_mbs[pstr->raw_mbs_idx + src_idx]; if (BE (pstr->trans != NULL, 0)) ch = pstr->trans [ch]; pstr->mbs[byte_idx] = ch; if (BE (pstr->offsets_needed != 0, 0)) pstr->offsets[byte_idx] = src_idx; ++src_idx; /* And also cast it to wide char. */ pstr->wcs[byte_idx++] = (wchar_t) ch; if (BE (mbclen == (size_t) -1, 0)) pstr->cur_state = prev_st; } else { /* The buffer doesn't have enough space, finish to build. */ pstr->cur_state = prev_st; break; } } pstr->valid_len = byte_idx; pstr->valid_raw_len = src_idx; return REG_NOERROR; } /* Skip characters until the index becomes greater than NEW_RAW_IDX. Return the index. */ static Idx re_string_skip_chars (re_string_t *pstr, Idx new_raw_idx, wint_t *last_wc) { mbstate_t prev_st; Idx rawbuf_idx; size_t mbclen; wint_t wc = WEOF; /* Skip the characters which are not necessary to check. */ for (rawbuf_idx = pstr->raw_mbs_idx + pstr->valid_raw_len; rawbuf_idx < new_raw_idx;) { wchar_t wc2; Idx remain_len = pstr->raw_len - rawbuf_idx; prev_st = pstr->cur_state; mbclen = __mbrtowc (&wc2, (const char *) pstr->raw_mbs + rawbuf_idx, remain_len, &pstr->cur_state); if (BE (mbclen == (size_t) -2 || mbclen == (size_t) -1 || mbclen == 0, 0)) { /* We treat these cases as a single byte character. */ if (mbclen == 0 || remain_len == 0) wc = L'\0'; else wc = *(unsigned char *) (pstr->raw_mbs + rawbuf_idx); mbclen = 1; pstr->cur_state = prev_st; } else wc = wc2; /* Then proceed the next character. */ rawbuf_idx += mbclen; } *last_wc = wc; return rawbuf_idx; } #endif /* RE_ENABLE_I18N */ /* Build the buffer PSTR->MBS, and apply the translation if we need. This function is used in case of REG_ICASE. */ static void build_upper_buffer (re_string_t *pstr) { Idx char_idx, end_idx; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; for (char_idx = pstr->valid_len; char_idx < end_idx; ++char_idx) { int ch = pstr->raw_mbs[pstr->raw_mbs_idx + char_idx]; if (BE (pstr->trans != NULL, 0)) ch = pstr->trans[ch]; pstr->mbs[char_idx] = toupper (ch); } pstr->valid_len = char_idx; pstr->valid_raw_len = char_idx; } /* Apply TRANS to the buffer in PSTR. */ static void re_string_translate_buffer (re_string_t *pstr) { Idx buf_idx, end_idx; end_idx = (pstr->bufs_len > pstr->len) ? pstr->len : pstr->bufs_len; for (buf_idx = pstr->valid_len; buf_idx < end_idx; ++buf_idx) { int ch = pstr->raw_mbs[pstr->raw_mbs_idx + buf_idx]; pstr->mbs[buf_idx] = pstr->trans[ch]; } pstr->valid_len = buf_idx; pstr->valid_raw_len = buf_idx; } /* This function re-construct the buffers. Concretely, convert to wide character in case of pstr->mb_cur_max > 1, convert to upper case in case of REG_ICASE, apply translation. */ static reg_errcode_t __attribute_warn_unused_result__ re_string_reconstruct (re_string_t *pstr, Idx idx, int eflags) { Idx offset; if (BE (pstr->raw_mbs_idx <= idx, 0)) offset = idx - pstr->raw_mbs_idx; else { /* Reset buffer. */ #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) memset (&pstr->cur_state, '\0', sizeof (mbstate_t)); #endif /* RE_ENABLE_I18N */ pstr->len = pstr->raw_len; pstr->stop = pstr->raw_stop; pstr->valid_len = 0; pstr->raw_mbs_idx = 0; pstr->valid_raw_len = 0; pstr->offsets_needed = 0; pstr->tip_context = ((eflags & REG_NOTBOL) ? CONTEXT_BEGBUF : CONTEXT_NEWLINE | CONTEXT_BEGBUF); if (!pstr->mbs_allocated) pstr->mbs = (unsigned char *) pstr->raw_mbs; offset = idx; } if (BE (offset != 0, 1)) { /* Should the already checked characters be kept? */ if (BE (offset < pstr->valid_raw_len, 1)) { /* Yes, move them to the front of the buffer. */ #ifdef RE_ENABLE_I18N if (BE (pstr->offsets_needed, 0)) { Idx low = 0, high = pstr->valid_len, mid; do { mid = (high + low) / 2; if (pstr->offsets[mid] > offset) high = mid; else if (pstr->offsets[mid] < offset) low = mid + 1; else break; } while (low < high); if (pstr->offsets[mid] < offset) ++mid; pstr->tip_context = re_string_context_at (pstr, mid - 1, eflags); /* This can be quite complicated, so handle specially only the common and easy case where the character with different length representation of lower and upper case is present at or after offset. */ if (pstr->valid_len > offset && mid == offset && pstr->offsets[mid] == offset) { memmove (pstr->wcs, pstr->wcs + offset, (pstr->valid_len - offset) * sizeof (wint_t)); memmove (pstr->mbs, pstr->mbs + offset, pstr->valid_len - offset); pstr->valid_len -= offset; pstr->valid_raw_len -= offset; for (low = 0; low < pstr->valid_len; low++) pstr->offsets[low] = pstr->offsets[low + offset] - offset; } else { /* Otherwise, just find out how long the partial multibyte character at offset is and fill it with WEOF/255. */ pstr->len = pstr->raw_len - idx + offset; pstr->stop = pstr->raw_stop - idx + offset; pstr->offsets_needed = 0; while (mid > 0 && pstr->offsets[mid - 1] == offset) --mid; while (mid < pstr->valid_len) if (pstr->wcs[mid] != WEOF) break; else ++mid; if (mid == pstr->valid_len) pstr->valid_len = 0; else { pstr->valid_len = pstr->offsets[mid] - offset; if (pstr->valid_len) { for (low = 0; low < pstr->valid_len; ++low) pstr->wcs[low] = WEOF; memset (pstr->mbs, 255, pstr->valid_len); } } pstr->valid_raw_len = pstr->valid_len; } } else #endif { pstr->tip_context = re_string_context_at (pstr, offset - 1, eflags); #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) memmove (pstr->wcs, pstr->wcs + offset, (pstr->valid_len - offset) * sizeof (wint_t)); #endif /* RE_ENABLE_I18N */ if (BE (pstr->mbs_allocated, 0)) memmove (pstr->mbs, pstr->mbs + offset, pstr->valid_len - offset); pstr->valid_len -= offset; pstr->valid_raw_len -= offset; #if defined DEBUG && DEBUG assert (pstr->valid_len > 0); #endif } } else { #ifdef RE_ENABLE_I18N /* No, skip all characters until IDX. */ Idx prev_valid_len = pstr->valid_len; if (BE (pstr->offsets_needed, 0)) { pstr->len = pstr->raw_len - idx + offset; pstr->stop = pstr->raw_stop - idx + offset; pstr->offsets_needed = 0; } #endif pstr->valid_len = 0; #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { Idx wcs_idx; wint_t wc = WEOF; if (pstr->is_utf8) { const unsigned char *raw, *p, *end; /* Special case UTF-8. Multi-byte chars start with any byte other than 0x80 - 0xbf. */ raw = pstr->raw_mbs + pstr->raw_mbs_idx; end = raw + (offset - pstr->mb_cur_max); if (end < pstr->raw_mbs) end = pstr->raw_mbs; p = raw + offset - 1; #ifdef _LIBC /* We know the wchar_t encoding is UCS4, so for the simple case, ASCII characters, skip the conversion step. */ if (isascii (*p) && BE (pstr->trans == NULL, 1)) { memset (&pstr->cur_state, '\0', sizeof (mbstate_t)); /* pstr->valid_len = 0; */ wc = (wchar_t) *p; } else #endif for (; p >= end; --p) if ((*p & 0xc0) != 0x80) { mbstate_t cur_state; wchar_t wc2; Idx mlen = raw + pstr->len - p; unsigned char buf[6]; size_t mbclen; const unsigned char *pp = p; if (BE (pstr->trans != NULL, 0)) { int i = mlen < 6 ? mlen : 6; while (--i >= 0) buf[i] = pstr->trans[p[i]]; pp = buf; } /* XXX Don't use mbrtowc, we know which conversion to use (UTF-8 -> UCS4). */ memset (&cur_state, 0, sizeof (cur_state)); mbclen = __mbrtowc (&wc2, (const char *) pp, mlen, &cur_state); if (raw + offset - p <= mbclen && mbclen < (size_t) -2) { memset (&pstr->cur_state, '\0', sizeof (mbstate_t)); pstr->valid_len = mbclen - (raw + offset - p); wc = wc2; } break; } } if (wc == WEOF) pstr->valid_len = re_string_skip_chars (pstr, idx, &wc) - idx; if (wc == WEOF) pstr->tip_context = re_string_context_at (pstr, prev_valid_len - 1, eflags); else pstr->tip_context = ((BE (pstr->word_ops_used != 0, 0) && IS_WIDE_WORD_CHAR (wc)) ? CONTEXT_WORD : ((IS_WIDE_NEWLINE (wc) && pstr->newline_anchor) ? CONTEXT_NEWLINE : 0)); if (BE (pstr->valid_len, 0)) { for (wcs_idx = 0; wcs_idx < pstr->valid_len; ++wcs_idx) pstr->wcs[wcs_idx] = WEOF; if (pstr->mbs_allocated) memset (pstr->mbs, 255, pstr->valid_len); } pstr->valid_raw_len = pstr->valid_len; } else #endif /* RE_ENABLE_I18N */ { int c = pstr->raw_mbs[pstr->raw_mbs_idx + offset - 1]; pstr->valid_raw_len = 0; if (pstr->trans) c = pstr->trans[c]; pstr->tip_context = (bitset_contain (pstr->word_char, c) ? CONTEXT_WORD : ((IS_NEWLINE (c) && pstr->newline_anchor) ? CONTEXT_NEWLINE : 0)); } } if (!BE (pstr->mbs_allocated, 0)) pstr->mbs += offset; } pstr->raw_mbs_idx = idx; pstr->len -= offset; pstr->stop -= offset; /* Then build the buffers. */ #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1) { if (pstr->icase) { reg_errcode_t ret = build_wcs_upper_buffer (pstr); if (BE (ret != REG_NOERROR, 0)) return ret; } else build_wcs_buffer (pstr); } else #endif /* RE_ENABLE_I18N */ if (BE (pstr->mbs_allocated, 0)) { if (pstr->icase) build_upper_buffer (pstr); else if (pstr->trans != NULL) re_string_translate_buffer (pstr); } else pstr->valid_len = pstr->len; pstr->cur_idx = 0; return REG_NOERROR; } static unsigned char __attribute__ ((pure)) re_string_peek_byte_case (const re_string_t *pstr, Idx idx) { int ch; Idx off; /* Handle the common (easiest) cases first. */ if (BE (!pstr->mbs_allocated, 1)) return re_string_peek_byte (pstr, idx); #ifdef RE_ENABLE_I18N if (pstr->mb_cur_max > 1 && ! re_string_is_single_byte_char (pstr, pstr->cur_idx + idx)) return re_string_peek_byte (pstr, idx); #endif off = pstr->cur_idx + idx; #ifdef RE_ENABLE_I18N if (pstr->offsets_needed) off = pstr->offsets[off]; #endif ch = pstr->raw_mbs[pstr->raw_mbs_idx + off]; #ifdef RE_ENABLE_I18N /* Ensure that e.g. for tr_TR.UTF-8 BACKSLASH DOTLESS SMALL LETTER I this function returns CAPITAL LETTER I instead of first byte of DOTLESS SMALL LETTER I. The latter would confuse the parser, since peek_byte_case doesn't advance cur_idx in any way. */ if (pstr->offsets_needed && !isascii (ch)) return re_string_peek_byte (pstr, idx); #endif return ch; } static unsigned char re_string_fetch_byte_case (re_string_t *pstr) { if (BE (!pstr->mbs_allocated, 1)) return re_string_fetch_byte (pstr); #ifdef RE_ENABLE_I18N if (pstr->offsets_needed) { Idx off; int ch; /* For tr_TR.UTF-8 [[:islower:]] there is [[: CAPITAL LETTER I WITH DOT lower:]] in mbs. Skip in that case the whole multi-byte character and return the original letter. On the other side, with [[: DOTLESS SMALL LETTER I return [[:I, as doing anything else would complicate things too much. */ if (!re_string_first_byte (pstr, pstr->cur_idx)) return re_string_fetch_byte (pstr); off = pstr->offsets[pstr->cur_idx]; ch = pstr->raw_mbs[pstr->raw_mbs_idx + off]; if (! isascii (ch)) return re_string_fetch_byte (pstr); re_string_skip_bytes (pstr, re_string_char_size_at (pstr, pstr->cur_idx)); return ch; } #endif return pstr->raw_mbs[pstr->raw_mbs_idx + pstr->cur_idx++]; } static void re_string_destruct (re_string_t *pstr) { #ifdef RE_ENABLE_I18N re_free (pstr->wcs); re_free (pstr->offsets); #endif /* RE_ENABLE_I18N */ if (pstr->mbs_allocated) re_free (pstr->mbs); } /* Return the context at IDX in INPUT. */ static unsigned int re_string_context_at (const re_string_t *input, Idx idx, int eflags) { int c; if (BE (idx < 0, 0)) /* In this case, we use the value stored in input->tip_context, since we can't know the character in input->mbs[-1] here. */ return input->tip_context; if (BE (idx == input->len, 0)) return ((eflags & REG_NOTEOL) ? CONTEXT_ENDBUF : CONTEXT_NEWLINE | CONTEXT_ENDBUF); #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1) { wint_t wc; Idx wc_idx = idx; while(input->wcs[wc_idx] == WEOF) { #if defined DEBUG && DEBUG /* It must not happen. */ assert (wc_idx >= 0); #endif --wc_idx; if (wc_idx < 0) return input->tip_context; } wc = input->wcs[wc_idx]; if (BE (input->word_ops_used != 0, 0) && IS_WIDE_WORD_CHAR (wc)) return CONTEXT_WORD; return (IS_WIDE_NEWLINE (wc) && input->newline_anchor ? CONTEXT_NEWLINE : 0); } else #endif { c = re_string_byte_at (input, idx); if (bitset_contain (input->word_char, c)) return CONTEXT_WORD; return IS_NEWLINE (c) && input->newline_anchor ? CONTEXT_NEWLINE : 0; } } /* Functions for set operation. */ static reg_errcode_t __attribute_warn_unused_result__ re_node_set_alloc (re_node_set *set, Idx size) { set->alloc = size; set->nelem = 0; set->elems = re_malloc (Idx, size); if (BE (set->elems == NULL, 0) && (MALLOC_0_IS_NONNULL || size != 0)) return REG_ESPACE; return REG_NOERROR; } static reg_errcode_t __attribute_warn_unused_result__ re_node_set_init_1 (re_node_set *set, Idx elem) { set->alloc = 1; set->nelem = 1; set->elems = re_malloc (Idx, 1); if (BE (set->elems == NULL, 0)) { set->alloc = set->nelem = 0; return REG_ESPACE; } set->elems[0] = elem; return REG_NOERROR; } static reg_errcode_t __attribute_warn_unused_result__ re_node_set_init_2 (re_node_set *set, Idx elem1, Idx elem2) { set->alloc = 2; set->elems = re_malloc (Idx, 2); if (BE (set->elems == NULL, 0)) return REG_ESPACE; if (elem1 == elem2) { set->nelem = 1; set->elems[0] = elem1; } else { set->nelem = 2; if (elem1 < elem2) { set->elems[0] = elem1; set->elems[1] = elem2; } else { set->elems[0] = elem2; set->elems[1] = elem1; } } return REG_NOERROR; } static reg_errcode_t __attribute_warn_unused_result__ re_node_set_init_copy (re_node_set *dest, const re_node_set *src) { dest->nelem = src->nelem; if (src->nelem > 0) { dest->alloc = dest->nelem; dest->elems = re_malloc (Idx, dest->alloc); if (BE (dest->elems == NULL, 0)) { dest->alloc = dest->nelem = 0; return REG_ESPACE; } memcpy (dest->elems, src->elems, src->nelem * sizeof (Idx)); } else re_node_set_init_empty (dest); return REG_NOERROR; } /* Calculate the intersection of the sets SRC1 and SRC2. And merge it to DEST. Return value indicate the error code or REG_NOERROR if succeeded. Note: We assume dest->elems is NULL, when dest->alloc is 0. */ static reg_errcode_t __attribute_warn_unused_result__ re_node_set_add_intersect (re_node_set *dest, const re_node_set *src1, const re_node_set *src2) { Idx i1, i2, is, id, delta, sbase; if (src1->nelem == 0 || src2->nelem == 0) return REG_NOERROR; /* We need dest->nelem + 2 * elems_in_intersection; this is a conservative estimate. */ if (src1->nelem + src2->nelem + dest->nelem > dest->alloc) { Idx new_alloc = src1->nelem + src2->nelem + dest->alloc; Idx *new_elems = re_realloc (dest->elems, Idx, new_alloc); if (BE (new_elems == NULL, 0)) return REG_ESPACE; dest->elems = new_elems; dest->alloc = new_alloc; } /* Find the items in the intersection of SRC1 and SRC2, and copy into the top of DEST those that are not already in DEST itself. */ sbase = dest->nelem + src1->nelem + src2->nelem; i1 = src1->nelem - 1; i2 = src2->nelem - 1; id = dest->nelem - 1; for (;;) { if (src1->elems[i1] == src2->elems[i2]) { /* Try to find the item in DEST. Maybe we could binary search? */ while (id >= 0 && dest->elems[id] > src1->elems[i1]) --id; if (id < 0 || dest->elems[id] != src1->elems[i1]) dest->elems[--sbase] = src1->elems[i1]; if (--i1 < 0 || --i2 < 0) break; } /* Lower the highest of the two items. */ else if (src1->elems[i1] < src2->elems[i2]) { if (--i2 < 0) break; } else { if (--i1 < 0) break; } } id = dest->nelem - 1; is = dest->nelem + src1->nelem + src2->nelem - 1; delta = is - sbase + 1; /* Now copy. When DELTA becomes zero, the remaining DEST elements are already in place; this is more or less the same loop that is in re_node_set_merge. */ dest->nelem += delta; if (delta > 0 && id >= 0) for (;;) { if (dest->elems[is] > dest->elems[id]) { /* Copy from the top. */ dest->elems[id + delta--] = dest->elems[is--]; if (delta == 0) break; } else { /* Slide from the bottom. */ dest->elems[id + delta] = dest->elems[id]; if (--id < 0) break; } } /* Copy remaining SRC elements. */ memcpy (dest->elems, dest->elems + sbase, delta * sizeof (Idx)); return REG_NOERROR; } /* Calculate the union set of the sets SRC1 and SRC2. And store it to DEST. Return value indicate the error code or REG_NOERROR if succeeded. */ static reg_errcode_t __attribute_warn_unused_result__ re_node_set_init_union (re_node_set *dest, const re_node_set *src1, const re_node_set *src2) { Idx i1, i2, id; if (src1 != NULL && src1->nelem > 0 && src2 != NULL && src2->nelem > 0) { dest->alloc = src1->nelem + src2->nelem; dest->elems = re_malloc (Idx, dest->alloc); if (BE (dest->elems == NULL, 0)) return REG_ESPACE; } else { if (src1 != NULL && src1->nelem > 0) return re_node_set_init_copy (dest, src1); else if (src2 != NULL && src2->nelem > 0) return re_node_set_init_copy (dest, src2); else re_node_set_init_empty (dest); return REG_NOERROR; } for (i1 = i2 = id = 0 ; i1 < src1->nelem && i2 < src2->nelem ;) { if (src1->elems[i1] > src2->elems[i2]) { dest->elems[id++] = src2->elems[i2++]; continue; } if (src1->elems[i1] == src2->elems[i2]) ++i2; dest->elems[id++] = src1->elems[i1++]; } if (i1 < src1->nelem) { memcpy (dest->elems + id, src1->elems + i1, (src1->nelem - i1) * sizeof (Idx)); id += src1->nelem - i1; } else if (i2 < src2->nelem) { memcpy (dest->elems + id, src2->elems + i2, (src2->nelem - i2) * sizeof (Idx)); id += src2->nelem - i2; } dest->nelem = id; return REG_NOERROR; } /* Calculate the union set of the sets DEST and SRC. And store it to DEST. Return value indicate the error code or REG_NOERROR if succeeded. */ static reg_errcode_t __attribute_warn_unused_result__ re_node_set_merge (re_node_set *dest, const re_node_set *src) { Idx is, id, sbase, delta; if (src == NULL || src->nelem == 0) return REG_NOERROR; if (dest->alloc < 2 * src->nelem + dest->nelem) { Idx new_alloc = 2 * (src->nelem + dest->alloc); Idx *new_buffer = re_realloc (dest->elems, Idx, new_alloc); if (BE (new_buffer == NULL, 0)) return REG_ESPACE; dest->elems = new_buffer; dest->alloc = new_alloc; } if (BE (dest->nelem == 0, 0)) { dest->nelem = src->nelem; memcpy (dest->elems, src->elems, src->nelem * sizeof (Idx)); return REG_NOERROR; } /* Copy into the top of DEST the items of SRC that are not found in DEST. Maybe we could binary search in DEST? */ for (sbase = dest->nelem + 2 * src->nelem, is = src->nelem - 1, id = dest->nelem - 1; is >= 0 && id >= 0; ) { if (dest->elems[id] == src->elems[is]) is--, id--; else if (dest->elems[id] < src->elems[is]) dest->elems[--sbase] = src->elems[is--]; else /* if (dest->elems[id] > src->elems[is]) */ --id; } if (is >= 0) { /* If DEST is exhausted, the remaining items of SRC must be unique. */ sbase -= is + 1; memcpy (dest->elems + sbase, src->elems, (is + 1) * sizeof (Idx)); } id = dest->nelem - 1; is = dest->nelem + 2 * src->nelem - 1; delta = is - sbase + 1; if (delta == 0) return REG_NOERROR; /* Now copy. When DELTA becomes zero, the remaining DEST elements are already in place. */ dest->nelem += delta; for (;;) { if (dest->elems[is] > dest->elems[id]) { /* Copy from the top. */ dest->elems[id + delta--] = dest->elems[is--]; if (delta == 0) break; } else { /* Slide from the bottom. */ dest->elems[id + delta] = dest->elems[id]; if (--id < 0) { /* Copy remaining SRC elements. */ memcpy (dest->elems, dest->elems + sbase, delta * sizeof (Idx)); break; } } } return REG_NOERROR; } /* Insert the new element ELEM to the re_node_set* SET. SET should not already have ELEM. Return true if successful. */ static bool __attribute_warn_unused_result__ re_node_set_insert (re_node_set *set, Idx elem) { Idx idx; /* In case the set is empty. */ if (set->alloc == 0) return BE (re_node_set_init_1 (set, elem) == REG_NOERROR, 1); if (BE (set->nelem, 0) == 0) { /* We already guaranteed above that set->alloc != 0. */ set->elems[0] = elem; ++set->nelem; return true; } /* Realloc if we need. */ if (set->alloc == set->nelem) { Idx *new_elems; set->alloc = set->alloc * 2; new_elems = re_realloc (set->elems, Idx, set->alloc); if (BE (new_elems == NULL, 0)) return false; set->elems = new_elems; } /* Move the elements which follows the new element. Test the first element separately to skip a check in the inner loop. */ if (elem < set->elems[0]) { idx = 0; for (idx = set->nelem; idx > 0; idx--) set->elems[idx] = set->elems[idx - 1]; } else { for (idx = set->nelem; set->elems[idx - 1] > elem; idx--) set->elems[idx] = set->elems[idx - 1]; } /* Insert the new element. */ set->elems[idx] = elem; ++set->nelem; return true; } /* Insert the new element ELEM to the re_node_set* SET. SET should not already have any element greater than or equal to ELEM. Return true if successful. */ static bool __attribute_warn_unused_result__ re_node_set_insert_last (re_node_set *set, Idx elem) { /* Realloc if we need. */ if (set->alloc == set->nelem) { Idx *new_elems; set->alloc = (set->alloc + 1) * 2; new_elems = re_realloc (set->elems, Idx, set->alloc); if (BE (new_elems == NULL, 0)) return false; set->elems = new_elems; } /* Insert the new element. */ set->elems[set->nelem++] = elem; return true; } /* Compare two node sets SET1 and SET2. Return true if SET1 and SET2 are equivalent. */ static bool __attribute__ ((pure)) re_node_set_compare (const re_node_set *set1, const re_node_set *set2) { Idx i; if (set1 == NULL || set2 == NULL || set1->nelem != set2->nelem) return false; for (i = set1->nelem ; --i >= 0 ; ) if (set1->elems[i] != set2->elems[i]) return false; return true; } /* Return (idx + 1) if SET contains the element ELEM, return 0 otherwise. */ static Idx __attribute__ ((pure)) re_node_set_contains (const re_node_set *set, Idx elem) { __re_size_t idx, right, mid; if (set->nelem <= 0) return 0; /* Binary search the element. */ idx = 0; right = set->nelem - 1; while (idx < right) { mid = (idx + right) / 2; if (set->elems[mid] < elem) idx = mid + 1; else right = mid; } return set->elems[idx] == elem ? idx + 1 : 0; } static void re_node_set_remove_at (re_node_set *set, Idx idx) { if (idx < 0 || idx >= set->nelem) return; --set->nelem; for (; idx < set->nelem; idx++) set->elems[idx] = set->elems[idx + 1]; } /* Add the token TOKEN to dfa->nodes, and return the index of the token. Or return -1 if an error occurred. */ static Idx re_dfa_add_node (re_dfa_t *dfa, re_token_t token) { if (BE (dfa->nodes_len >= dfa->nodes_alloc, 0)) { size_t new_nodes_alloc = dfa->nodes_alloc * 2; Idx *new_nexts, *new_indices; re_node_set *new_edests, *new_eclosures; re_token_t *new_nodes; /* Avoid overflows in realloc. */ const size_t max_object_size = MAX (sizeof (re_token_t), MAX (sizeof (re_node_set), sizeof (Idx))); if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) < new_nodes_alloc, 0)) return -1; new_nodes = re_realloc (dfa->nodes, re_token_t, new_nodes_alloc); if (BE (new_nodes == NULL, 0)) return -1; dfa->nodes = new_nodes; new_nexts = re_realloc (dfa->nexts, Idx, new_nodes_alloc); new_indices = re_realloc (dfa->org_indices, Idx, new_nodes_alloc); new_edests = re_realloc (dfa->edests, re_node_set, new_nodes_alloc); new_eclosures = re_realloc (dfa->eclosures, re_node_set, new_nodes_alloc); if (BE (new_nexts == NULL || new_indices == NULL || new_edests == NULL || new_eclosures == NULL, 0)) { re_free (new_nexts); re_free (new_indices); re_free (new_edests); re_free (new_eclosures); return -1; } dfa->nexts = new_nexts; dfa->org_indices = new_indices; dfa->edests = new_edests; dfa->eclosures = new_eclosures; dfa->nodes_alloc = new_nodes_alloc; } dfa->nodes[dfa->nodes_len] = token; dfa->nodes[dfa->nodes_len].constraint = 0; #ifdef RE_ENABLE_I18N dfa->nodes[dfa->nodes_len].accept_mb = ((token.type == OP_PERIOD && dfa->mb_cur_max > 1) || token.type == COMPLEX_BRACKET); #endif dfa->nexts[dfa->nodes_len] = -1; re_node_set_init_empty (dfa->edests + dfa->nodes_len); re_node_set_init_empty (dfa->eclosures + dfa->nodes_len); return dfa->nodes_len++; } static re_hashval_t calc_state_hash (const re_node_set *nodes, unsigned int context) { re_hashval_t hash = nodes->nelem + context; Idx i; for (i = 0 ; i < nodes->nelem ; i++) hash += nodes->elems[i]; return hash; } /* Search for the state whose node_set is equivalent to NODES. Return the pointer to the state, if we found it in the DFA. Otherwise create the new one and return it. In case of an error return NULL and set the error code in ERR. Note: - We assume NULL as the invalid state, then it is possible that return value is NULL and ERR is REG_NOERROR. - We never return non-NULL value in case of any errors, it is for optimization. */ static re_dfastate_t * __attribute_warn_unused_result__ re_acquire_state (reg_errcode_t *err, const re_dfa_t *dfa, const re_node_set *nodes) { re_hashval_t hash; re_dfastate_t *new_state; struct re_state_table_entry *spot; Idx i; #if defined GCC_LINT || defined lint /* Suppress bogus uninitialized-variable warnings. */ *err = REG_NOERROR; #endif if (BE (nodes->nelem == 0, 0)) { *err = REG_NOERROR; return NULL; } hash = calc_state_hash (nodes, 0); spot = dfa->state_table + (hash & dfa->state_hash_mask); for (i = 0 ; i < spot->num ; i++) { re_dfastate_t *state = spot->array[i]; if (hash != state->hash) continue; if (re_node_set_compare (&state->nodes, nodes)) return state; } /* There are no appropriate state in the dfa, create the new one. */ new_state = create_ci_newstate (dfa, nodes, hash); if (BE (new_state == NULL, 0)) *err = REG_ESPACE; return new_state; } /* Search for the state whose node_set is equivalent to NODES and whose context is equivalent to CONTEXT. Return the pointer to the state, if we found it in the DFA. Otherwise create the new one and return it. In case of an error return NULL and set the error code in ERR. Note: - We assume NULL as the invalid state, then it is possible that return value is NULL and ERR is REG_NOERROR. - We never return non-NULL value in case of any errors, it is for optimization. */ static re_dfastate_t * __attribute_warn_unused_result__ re_acquire_state_context (reg_errcode_t *err, const re_dfa_t *dfa, const re_node_set *nodes, unsigned int context) { re_hashval_t hash; re_dfastate_t *new_state; struct re_state_table_entry *spot; Idx i; #if defined GCC_LINT || defined lint /* Suppress bogus uninitialized-variable warnings. */ *err = REG_NOERROR; #endif if (nodes->nelem == 0) { *err = REG_NOERROR; return NULL; } hash = calc_state_hash (nodes, context); spot = dfa->state_table + (hash & dfa->state_hash_mask); for (i = 0 ; i < spot->num ; i++) { re_dfastate_t *state = spot->array[i]; if (state->hash == hash && state->context == context && re_node_set_compare (state->entrance_nodes, nodes)) return state; } /* There are no appropriate state in 'dfa', create the new one. */ new_state = create_cd_newstate (dfa, nodes, context, hash); if (BE (new_state == NULL, 0)) *err = REG_ESPACE; return new_state; } /* Finish initialization of the new state NEWSTATE, and using its hash value HASH put in the appropriate bucket of DFA's state table. Return value indicates the error code if failed. */ static reg_errcode_t __attribute_warn_unused_result__ register_state (const re_dfa_t *dfa, re_dfastate_t *newstate, re_hashval_t hash) { struct re_state_table_entry *spot; reg_errcode_t err; Idx i; newstate->hash = hash; err = re_node_set_alloc (&newstate->non_eps_nodes, newstate->nodes.nelem); if (BE (err != REG_NOERROR, 0)) return REG_ESPACE; for (i = 0; i < newstate->nodes.nelem; i++) { Idx elem = newstate->nodes.elems[i]; if (!IS_EPSILON_NODE (dfa->nodes[elem].type)) if (! re_node_set_insert_last (&newstate->non_eps_nodes, elem)) return REG_ESPACE; } spot = dfa->state_table + (hash & dfa->state_hash_mask); if (BE (spot->alloc <= spot->num, 0)) { Idx new_alloc = 2 * spot->num + 2; re_dfastate_t **new_array = re_realloc (spot->array, re_dfastate_t *, new_alloc); if (BE (new_array == NULL, 0)) return REG_ESPACE; spot->array = new_array; spot->alloc = new_alloc; } spot->array[spot->num++] = newstate; return REG_NOERROR; } static void free_state (re_dfastate_t *state) { re_node_set_free (&state->non_eps_nodes); re_node_set_free (&state->inveclosure); if (state->entrance_nodes != &state->nodes) { re_node_set_free (state->entrance_nodes); re_free (state->entrance_nodes); } re_node_set_free (&state->nodes); re_free (state->word_trtable); re_free (state->trtable); re_free (state); } /* Create the new state which is independent of contexts. Return the new state if succeeded, otherwise return NULL. */ static re_dfastate_t * __attribute_warn_unused_result__ create_ci_newstate (const re_dfa_t *dfa, const re_node_set *nodes, re_hashval_t hash) { Idx i; reg_errcode_t err; re_dfastate_t *newstate; newstate = (re_dfastate_t *) calloc (sizeof (re_dfastate_t), 1); if (BE (newstate == NULL, 0)) return NULL; err = re_node_set_init_copy (&newstate->nodes, nodes); if (BE (err != REG_NOERROR, 0)) { re_free (newstate); return NULL; } newstate->entrance_nodes = &newstate->nodes; for (i = 0 ; i < nodes->nelem ; i++) { re_token_t *node = dfa->nodes + nodes->elems[i]; re_token_type_t type = node->type; if (type == CHARACTER && !node->constraint) continue; #ifdef RE_ENABLE_I18N newstate->accept_mb |= node->accept_mb; #endif /* RE_ENABLE_I18N */ /* If the state has the halt node, the state is a halt state. */ if (type == END_OF_RE) newstate->halt = 1; else if (type == OP_BACK_REF) newstate->has_backref = 1; else if (type == ANCHOR || node->constraint) newstate->has_constraint = 1; } err = register_state (dfa, newstate, hash); if (BE (err != REG_NOERROR, 0)) { free_state (newstate); newstate = NULL; } return newstate; } /* Create the new state which is depend on the context CONTEXT. Return the new state if succeeded, otherwise return NULL. */ static re_dfastate_t * __attribute_warn_unused_result__ create_cd_newstate (const re_dfa_t *dfa, const re_node_set *nodes, unsigned int context, re_hashval_t hash) { Idx i, nctx_nodes = 0; reg_errcode_t err; re_dfastate_t *newstate; newstate = (re_dfastate_t *) calloc (sizeof (re_dfastate_t), 1); if (BE (newstate == NULL, 0)) return NULL; err = re_node_set_init_copy (&newstate->nodes, nodes); if (BE (err != REG_NOERROR, 0)) { re_free (newstate); return NULL; } newstate->context = context; newstate->entrance_nodes = &newstate->nodes; for (i = 0 ; i < nodes->nelem ; i++) { re_token_t *node = dfa->nodes + nodes->elems[i]; re_token_type_t type = node->type; unsigned int constraint = node->constraint; if (type == CHARACTER && !constraint) continue; #ifdef RE_ENABLE_I18N newstate->accept_mb |= node->accept_mb; #endif /* RE_ENABLE_I18N */ /* If the state has the halt node, the state is a halt state. */ if (type == END_OF_RE) newstate->halt = 1; else if (type == OP_BACK_REF) newstate->has_backref = 1; if (constraint) { if (newstate->entrance_nodes == &newstate->nodes) { newstate->entrance_nodes = re_malloc (re_node_set, 1); if (BE (newstate->entrance_nodes == NULL, 0)) { free_state (newstate); return NULL; } if (re_node_set_init_copy (newstate->entrance_nodes, nodes) != REG_NOERROR) return NULL; nctx_nodes = 0; newstate->has_constraint = 1; } if (NOT_SATISFY_PREV_CONSTRAINT (constraint,context)) { re_node_set_remove_at (&newstate->nodes, i - nctx_nodes); ++nctx_nodes; } } } err = register_state (dfa, newstate, hash); if (BE (err != REG_NOERROR, 0)) { free_state (newstate); newstate = NULL; } return newstate; } gnuastro-0.5/bootstrapped/lib/regex.c0000644000175000017500000000615413217200021014665 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _LIBC # include # if (__GNUC__ == 4 && 6 <= __GNUC_MINOR__) || 4 < __GNUC__ # pragma GCC diagnostic ignored "-Wsuggest-attribute=pure" # endif # if (__GNUC__ == 4 && 3 <= __GNUC_MINOR__) || 4 < __GNUC__ # pragma GCC diagnostic ignored "-Wold-style-definition" # pragma GCC diagnostic ignored "-Wtype-limits" # endif #endif /* Make sure no one compiles this code with a C++ compiler. */ #if defined __cplusplus && defined _LIBC # error "This is C code, use a C compiler" #endif #ifdef _LIBC /* We have to keep the namespace clean. */ # define regfree(preg) __regfree (preg) # define regexec(pr, st, nm, pm, ef) __regexec (pr, st, nm, pm, ef) # define regcomp(preg, pattern, cflags) __regcomp (preg, pattern, cflags) # define regerror(errcode, preg, errbuf, errbuf_size) \ __regerror(errcode, preg, errbuf, errbuf_size) # define re_set_registers(bu, re, nu, st, en) \ __re_set_registers (bu, re, nu, st, en) # define re_match_2(bufp, string1, size1, string2, size2, pos, regs, stop) \ __re_match_2 (bufp, string1, size1, string2, size2, pos, regs, stop) # define re_match(bufp, string, size, pos, regs) \ __re_match (bufp, string, size, pos, regs) # define re_search(bufp, string, size, startpos, range, regs) \ __re_search (bufp, string, size, startpos, range, regs) # define re_compile_pattern(pattern, length, bufp) \ __re_compile_pattern (pattern, length, bufp) # define re_set_syntax(syntax) __re_set_syntax (syntax) # define re_search_2(bufp, st1, s1, st2, s2, startpos, range, regs, stop) \ __re_search_2 (bufp, st1, s1, st2, s2, startpos, range, regs, stop) # define re_compile_fastmap(bufp) __re_compile_fastmap (bufp) # include "../locale/localeinfo.h" #endif /* On some systems, limits.h sets RE_DUP_MAX to a lower value than GNU regex allows. Include it before , which correctly #undefs RE_DUP_MAX and sets it to the right value. */ #include #include #include "regex_internal.h" #include "regex_internal.c" #include "regcomp.c" #include "regexec.c" /* Binary backward compatibility. */ #if _LIBC # include # if SHLIB_COMPAT (libc, GLIBC_2_0, GLIBC_2_3) link_warning (re_max_failures, "the 're_max_failures' variable is obsolete and will go away.") int re_max_failures = 2000; # endif #endif gnuastro-0.5/bootstrapped/lib/regcomp.c0000644000175000017500000033554213217200021015215 00000000000000/* Extended regular expression matching and search library. Copyright (C) 2002-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Contributed by Isamu Hasegawa . The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifdef _LIBC # include #endif static reg_errcode_t re_compile_internal (regex_t *preg, const char * pattern, size_t length, reg_syntax_t syntax); static void re_compile_fastmap_iter (regex_t *bufp, const re_dfastate_t *init_state, char *fastmap); static reg_errcode_t init_dfa (re_dfa_t *dfa, size_t pat_len); #ifdef RE_ENABLE_I18N static void free_charset (re_charset_t *cset); #endif /* RE_ENABLE_I18N */ static void free_workarea_compile (regex_t *preg); static reg_errcode_t create_initial_state (re_dfa_t *dfa); #ifdef RE_ENABLE_I18N static void optimize_utf8 (re_dfa_t *dfa); #endif static reg_errcode_t analyze (regex_t *preg); static reg_errcode_t preorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra); static reg_errcode_t postorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra); static reg_errcode_t optimize_subexps (void *extra, bin_tree_t *node); static reg_errcode_t lower_subexps (void *extra, bin_tree_t *node); static bin_tree_t *lower_subexp (reg_errcode_t *err, regex_t *preg, bin_tree_t *node); static reg_errcode_t calc_first (void *extra, bin_tree_t *node); static reg_errcode_t calc_next (void *extra, bin_tree_t *node); static reg_errcode_t link_nfa_nodes (void *extra, bin_tree_t *node); static Idx duplicate_node (re_dfa_t *dfa, Idx org_idx, unsigned int constraint); static Idx search_duplicated_node (const re_dfa_t *dfa, Idx org_node, unsigned int constraint); static reg_errcode_t calc_eclosure (re_dfa_t *dfa); static reg_errcode_t calc_eclosure_iter (re_node_set *new_set, re_dfa_t *dfa, Idx node, bool root); static reg_errcode_t calc_inveclosure (re_dfa_t *dfa); static Idx fetch_number (re_string_t *input, re_token_t *token, reg_syntax_t syntax); static int peek_token (re_token_t *token, re_string_t *input, reg_syntax_t syntax); static bin_tree_t *parse (re_string_t *regexp, regex_t *preg, reg_syntax_t syntax, reg_errcode_t *err); static bin_tree_t *parse_reg_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_branch (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_expression (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_sub_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err); static bin_tree_t *parse_dup_op (bin_tree_t *dup_elem, re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err); static bin_tree_t *parse_bracket_exp (re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err); static reg_errcode_t parse_bracket_element (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token, int token_len, re_dfa_t *dfa, reg_syntax_t syntax, bool accept_hyphen); static reg_errcode_t parse_bracket_symbol (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token); #ifdef RE_ENABLE_I18N static reg_errcode_t build_equiv_class (bitset_t sbcset, re_charset_t *mbcset, Idx *equiv_class_alloc, const unsigned char *name); static reg_errcode_t build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, re_charset_t *mbcset, Idx *char_class_alloc, const char *class_name, reg_syntax_t syntax); #else /* not RE_ENABLE_I18N */ static reg_errcode_t build_equiv_class (bitset_t sbcset, const unsigned char *name); static reg_errcode_t build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, const char *class_name, reg_syntax_t syntax); #endif /* not RE_ENABLE_I18N */ static bin_tree_t *build_charclass_op (re_dfa_t *dfa, RE_TRANSLATE_TYPE trans, const char *class_name, const char *extra, bool non_match, reg_errcode_t *err); static bin_tree_t *create_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, re_token_type_t type); static bin_tree_t *create_token_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, const re_token_t *token); static bin_tree_t *duplicate_tree (const bin_tree_t *src, re_dfa_t *dfa); static void free_token (re_token_t *node); static reg_errcode_t free_tree (void *extra, bin_tree_t *node); static reg_errcode_t mark_opt_subexp (void *extra, bin_tree_t *node); /* This table gives an error message for each of the error codes listed in regex.h. Obviously the order here has to be same as there. POSIX doesn't require that we do anything for REG_NOERROR, but why not be nice? */ static const char __re_error_msgid[] = { #define REG_NOERROR_IDX 0 gettext_noop ("Success") /* REG_NOERROR */ "\0" #define REG_NOMATCH_IDX (REG_NOERROR_IDX + sizeof "Success") gettext_noop ("No match") /* REG_NOMATCH */ "\0" #define REG_BADPAT_IDX (REG_NOMATCH_IDX + sizeof "No match") gettext_noop ("Invalid regular expression") /* REG_BADPAT */ "\0" #define REG_ECOLLATE_IDX (REG_BADPAT_IDX + sizeof "Invalid regular expression") gettext_noop ("Invalid collation character") /* REG_ECOLLATE */ "\0" #define REG_ECTYPE_IDX (REG_ECOLLATE_IDX + sizeof "Invalid collation character") gettext_noop ("Invalid character class name") /* REG_ECTYPE */ "\0" #define REG_EESCAPE_IDX (REG_ECTYPE_IDX + sizeof "Invalid character class name") gettext_noop ("Trailing backslash") /* REG_EESCAPE */ "\0" #define REG_ESUBREG_IDX (REG_EESCAPE_IDX + sizeof "Trailing backslash") gettext_noop ("Invalid back reference") /* REG_ESUBREG */ "\0" #define REG_EBRACK_IDX (REG_ESUBREG_IDX + sizeof "Invalid back reference") gettext_noop ("Unmatched [, [^, [:, [., or [=") /* REG_EBRACK */ "\0" #define REG_EPAREN_IDX (REG_EBRACK_IDX + sizeof "Unmatched [, [^, [:, [., or [=") gettext_noop ("Unmatched ( or \\(") /* REG_EPAREN */ "\0" #define REG_EBRACE_IDX (REG_EPAREN_IDX + sizeof "Unmatched ( or \\(") gettext_noop ("Unmatched \\{") /* REG_EBRACE */ "\0" #define REG_BADBR_IDX (REG_EBRACE_IDX + sizeof "Unmatched \\{") gettext_noop ("Invalid content of \\{\\}") /* REG_BADBR */ "\0" #define REG_ERANGE_IDX (REG_BADBR_IDX + sizeof "Invalid content of \\{\\}") gettext_noop ("Invalid range end") /* REG_ERANGE */ "\0" #define REG_ESPACE_IDX (REG_ERANGE_IDX + sizeof "Invalid range end") gettext_noop ("Memory exhausted") /* REG_ESPACE */ "\0" #define REG_BADRPT_IDX (REG_ESPACE_IDX + sizeof "Memory exhausted") gettext_noop ("Invalid preceding regular expression") /* REG_BADRPT */ "\0" #define REG_EEND_IDX (REG_BADRPT_IDX + sizeof "Invalid preceding regular expression") gettext_noop ("Premature end of regular expression") /* REG_EEND */ "\0" #define REG_ESIZE_IDX (REG_EEND_IDX + sizeof "Premature end of regular expression") gettext_noop ("Regular expression too big") /* REG_ESIZE */ "\0" #define REG_ERPAREN_IDX (REG_ESIZE_IDX + sizeof "Regular expression too big") gettext_noop ("Unmatched ) or \\)") /* REG_ERPAREN */ }; static const size_t __re_error_msgid_idx[] = { REG_NOERROR_IDX, REG_NOMATCH_IDX, REG_BADPAT_IDX, REG_ECOLLATE_IDX, REG_ECTYPE_IDX, REG_EESCAPE_IDX, REG_ESUBREG_IDX, REG_EBRACK_IDX, REG_EPAREN_IDX, REG_EBRACE_IDX, REG_BADBR_IDX, REG_ERANGE_IDX, REG_ESPACE_IDX, REG_BADRPT_IDX, REG_EEND_IDX, REG_ESIZE_IDX, REG_ERPAREN_IDX }; /* Entry points for GNU code. */ /* re_compile_pattern is the GNU regular expression compiler: it compiles PATTERN (of length LENGTH) and puts the result in BUFP. Returns 0 if the pattern was valid, otherwise an error string. Assumes the 'allocated' (and perhaps 'buffer') and 'translate' fields are set in BUFP on entry. */ const char * re_compile_pattern (const char *pattern, size_t length, struct re_pattern_buffer *bufp) { reg_errcode_t ret; /* And GNU code determines whether or not to get register information by passing null for the REGS argument to re_match, etc., not by setting no_sub, unless RE_NO_SUB is set. */ bufp->no_sub = !!(re_syntax_options & RE_NO_SUB); /* Match anchors at newline. */ bufp->newline_anchor = 1; ret = re_compile_internal (bufp, pattern, length, re_syntax_options); if (!ret) return NULL; return gettext (__re_error_msgid + __re_error_msgid_idx[(int) ret]); } #ifdef _LIBC weak_alias (__re_compile_pattern, re_compile_pattern) #endif /* Set by 're_set_syntax' to the current regexp syntax to recognize. Can also be assigned to arbitrarily: each pattern buffer stores its own syntax, so it can be changed between regex compilations. */ /* This has no initializer because initialized variables in Emacs become read-only after dumping. */ reg_syntax_t re_syntax_options; /* Specify the precise syntax of regexps for compilation. This provides for compatibility for various utilities which historically have different, incompatible syntaxes. The argument SYNTAX is a bit mask comprised of the various bits defined in regex.h. We return the old syntax. */ reg_syntax_t re_set_syntax (reg_syntax_t syntax) { reg_syntax_t ret = re_syntax_options; re_syntax_options = syntax; return ret; } #ifdef _LIBC weak_alias (__re_set_syntax, re_set_syntax) #endif int re_compile_fastmap (struct re_pattern_buffer *bufp) { re_dfa_t *dfa = bufp->buffer; char *fastmap = bufp->fastmap; memset (fastmap, '\0', sizeof (char) * SBC_MAX); re_compile_fastmap_iter (bufp, dfa->init_state, fastmap); if (dfa->init_state != dfa->init_state_word) re_compile_fastmap_iter (bufp, dfa->init_state_word, fastmap); if (dfa->init_state != dfa->init_state_nl) re_compile_fastmap_iter (bufp, dfa->init_state_nl, fastmap); if (dfa->init_state != dfa->init_state_begbuf) re_compile_fastmap_iter (bufp, dfa->init_state_begbuf, fastmap); bufp->fastmap_accurate = 1; return 0; } #ifdef _LIBC weak_alias (__re_compile_fastmap, re_compile_fastmap) #endif static inline void __attribute__ ((always_inline)) re_set_fastmap (char *fastmap, bool icase, int ch) { fastmap[ch] = 1; if (icase) fastmap[tolower (ch)] = 1; } /* Helper function for re_compile_fastmap. Compile fastmap for the initial_state INIT_STATE. */ static void re_compile_fastmap_iter (regex_t *bufp, const re_dfastate_t *init_state, char *fastmap) { re_dfa_t *dfa = bufp->buffer; Idx node_cnt; bool icase = (dfa->mb_cur_max == 1 && (bufp->syntax & RE_ICASE)); for (node_cnt = 0; node_cnt < init_state->nodes.nelem; ++node_cnt) { Idx node = init_state->nodes.elems[node_cnt]; re_token_type_t type = dfa->nodes[node].type; if (type == CHARACTER) { re_set_fastmap (fastmap, icase, dfa->nodes[node].opr.c); #ifdef RE_ENABLE_I18N if ((bufp->syntax & RE_ICASE) && dfa->mb_cur_max > 1) { unsigned char buf[MB_LEN_MAX]; unsigned char *p; wchar_t wc; mbstate_t state; p = buf; *p++ = dfa->nodes[node].opr.c; while (++node < dfa->nodes_len && dfa->nodes[node].type == CHARACTER && dfa->nodes[node].mb_partial) *p++ = dfa->nodes[node].opr.c; memset (&state, '\0', sizeof (state)); if (__mbrtowc (&wc, (const char *) buf, p - buf, &state) == p - buf && (__wcrtomb ((char *) buf, __towlower (wc), &state) != (size_t) -1)) re_set_fastmap (fastmap, false, buf[0]); } #endif } else if (type == SIMPLE_BRACKET) { int i, ch; for (i = 0, ch = 0; i < BITSET_WORDS; ++i) { int j; bitset_word_t w = dfa->nodes[node].opr.sbcset[i]; for (j = 0; j < BITSET_WORD_BITS; ++j, ++ch) if (w & ((bitset_word_t) 1 << j)) re_set_fastmap (fastmap, icase, ch); } } #ifdef RE_ENABLE_I18N else if (type == COMPLEX_BRACKET) { re_charset_t *cset = dfa->nodes[node].opr.mbcset; Idx i; # ifdef _LIBC /* See if we have to try all bytes which start multiple collation elements. e.g. In da_DK, we want to catch 'a' since "aa" is a valid collation element, and don't catch 'b' since 'b' is the only collation element which starts from 'b' (and it is caught by SIMPLE_BRACKET). */ if (_NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES) != 0 && (cset->ncoll_syms || cset->nranges)) { const int32_t *table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); for (i = 0; i < SBC_MAX; ++i) if (table[i] < 0) re_set_fastmap (fastmap, icase, i); } # endif /* _LIBC */ /* See if we have to start the match at all multibyte characters, i.e. where we would not find an invalid sequence. This only applies to multibyte character sets; for single byte character sets, the SIMPLE_BRACKET again suffices. */ if (dfa->mb_cur_max > 1 && (cset->nchar_classes || cset->non_match || cset->nranges # ifdef _LIBC || cset->nequiv_classes # endif /* _LIBC */ )) { unsigned char c = 0; do { mbstate_t mbs; memset (&mbs, 0, sizeof (mbs)); if (__mbrtowc (NULL, (char *) &c, 1, &mbs) == (size_t) -2) re_set_fastmap (fastmap, false, (int) c); } while (++c != 0); } else { /* ... Else catch all bytes which can start the mbchars. */ for (i = 0; i < cset->nmbchars; ++i) { char buf[256]; mbstate_t state; memset (&state, '\0', sizeof (state)); if (__wcrtomb (buf, cset->mbchars[i], &state) != (size_t) -1) re_set_fastmap (fastmap, icase, *(unsigned char *) buf); if ((bufp->syntax & RE_ICASE) && dfa->mb_cur_max > 1) { if (__wcrtomb (buf, __towlower (cset->mbchars[i]), &state) != (size_t) -1) re_set_fastmap (fastmap, false, *(unsigned char *) buf); } } } } #endif /* RE_ENABLE_I18N */ else if (type == OP_PERIOD #ifdef RE_ENABLE_I18N || type == OP_UTF8_PERIOD #endif /* RE_ENABLE_I18N */ || type == END_OF_RE) { memset (fastmap, '\1', sizeof (char) * SBC_MAX); if (type == END_OF_RE) bufp->can_be_null = 1; return; } } } /* Entry point for POSIX code. */ /* regcomp takes a regular expression as a string and compiles it. PREG is a regex_t *. We do not expect any fields to be initialized, since POSIX says we shouldn't. Thus, we set 'buffer' to the compiled pattern; 'used' to the length of the compiled pattern; 'syntax' to RE_SYNTAX_POSIX_EXTENDED if the REG_EXTENDED bit in CFLAGS is set; otherwise, to RE_SYNTAX_POSIX_BASIC; 'newline_anchor' to REG_NEWLINE being set in CFLAGS; 'fastmap' to an allocated space for the fastmap; 'fastmap_accurate' to zero; 're_nsub' to the number of subexpressions in PATTERN. PATTERN is the address of the pattern string. CFLAGS is a series of bits which affect compilation. If REG_EXTENDED is set, we use POSIX extended syntax; otherwise, we use POSIX basic syntax. If REG_NEWLINE is set, then . and [^...] don't match newline. Also, regexec will try a match beginning after every newline. If REG_ICASE is set, then we considers upper- and lowercase versions of letters to be equivalent when matching. If REG_NOSUB is set, then when PREG is passed to regexec, that routine will report only success or failure, and nothing about the registers. It returns 0 if it succeeds, nonzero if it doesn't. (See regex.h for the return codes and their meanings.) */ int regcomp (regex_t *_Restrict_ preg, const char *_Restrict_ pattern, int cflags) { reg_errcode_t ret; reg_syntax_t syntax = ((cflags & REG_EXTENDED) ? RE_SYNTAX_POSIX_EXTENDED : RE_SYNTAX_POSIX_BASIC); preg->buffer = NULL; preg->allocated = 0; preg->used = 0; /* Try to allocate space for the fastmap. */ preg->fastmap = re_malloc (char, SBC_MAX); if (BE (preg->fastmap == NULL, 0)) return REG_ESPACE; syntax |= (cflags & REG_ICASE) ? RE_ICASE : 0; /* If REG_NEWLINE is set, newlines are treated differently. */ if (cflags & REG_NEWLINE) { /* REG_NEWLINE implies neither . nor [^...] match newline. */ syntax &= ~RE_DOT_NEWLINE; syntax |= RE_HAT_LISTS_NOT_NEWLINE; /* It also changes the matching behavior. */ preg->newline_anchor = 1; } else preg->newline_anchor = 0; preg->no_sub = !!(cflags & REG_NOSUB); preg->translate = NULL; ret = re_compile_internal (preg, pattern, strlen (pattern), syntax); /* POSIX doesn't distinguish between an unmatched open-group and an unmatched close-group: both are REG_EPAREN. */ if (ret == REG_ERPAREN) ret = REG_EPAREN; /* We have already checked preg->fastmap != NULL. */ if (BE (ret == REG_NOERROR, 1)) /* Compute the fastmap now, since regexec cannot modify the pattern buffer. This function never fails in this implementation. */ (void) re_compile_fastmap (preg); else { /* Some error occurred while compiling the expression. */ re_free (preg->fastmap); preg->fastmap = NULL; } return (int) ret; } #ifdef _LIBC libc_hidden_def (__regcomp) weak_alias (__regcomp, regcomp) #endif /* Returns a message corresponding to an error code, ERRCODE, returned from either regcomp or regexec. We don't use PREG here. */ size_t regerror (int errcode, const regex_t *_Restrict_ preg, char *_Restrict_ errbuf, size_t errbuf_size) { const char *msg; size_t msg_size; if (BE (errcode < 0 || errcode >= (int) (sizeof (__re_error_msgid_idx) / sizeof (__re_error_msgid_idx[0])), 0)) /* Only error codes returned by the rest of the code should be passed to this routine. If we are given anything else, or if other regex code generates an invalid error code, then the program has a bug. Dump core so we can fix it. */ abort (); msg = gettext (__re_error_msgid + __re_error_msgid_idx[errcode]); msg_size = strlen (msg) + 1; /* Includes the null. */ if (BE (errbuf_size != 0, 1)) { size_t cpy_size = msg_size; if (BE (msg_size > errbuf_size, 0)) { cpy_size = errbuf_size - 1; errbuf[cpy_size] = '\0'; } memcpy (errbuf, msg, cpy_size); } return msg_size; } #ifdef _LIBC weak_alias (__regerror, regerror) #endif #ifdef RE_ENABLE_I18N /* This static array is used for the map to single-byte characters when UTF-8 is used. Otherwise we would allocate memory just to initialize it the same all the time. UTF-8 is the preferred encoding so this is a worthwhile optimization. */ static const bitset_t utf8_sb_map = { /* Set the first 128 bits. */ # if defined __GNUC__ && !defined __STRICT_ANSI__ [0 ... 0x80 / BITSET_WORD_BITS - 1] = BITSET_WORD_MAX # else # if 4 * BITSET_WORD_BITS < ASCII_CHARS # error "bitset_word_t is narrower than 32 bits" # elif 3 * BITSET_WORD_BITS < ASCII_CHARS BITSET_WORD_MAX, BITSET_WORD_MAX, BITSET_WORD_MAX, # elif 2 * BITSET_WORD_BITS < ASCII_CHARS BITSET_WORD_MAX, BITSET_WORD_MAX, # elif 1 * BITSET_WORD_BITS < ASCII_CHARS BITSET_WORD_MAX, # endif (BITSET_WORD_MAX >> (SBC_MAX % BITSET_WORD_BITS == 0 ? 0 : BITSET_WORD_BITS - SBC_MAX % BITSET_WORD_BITS)) # endif }; #endif static void free_dfa_content (re_dfa_t *dfa) { Idx i, j; if (dfa->nodes) for (i = 0; i < dfa->nodes_len; ++i) free_token (dfa->nodes + i); re_free (dfa->nexts); for (i = 0; i < dfa->nodes_len; ++i) { if (dfa->eclosures != NULL) re_node_set_free (dfa->eclosures + i); if (dfa->inveclosures != NULL) re_node_set_free (dfa->inveclosures + i); if (dfa->edests != NULL) re_node_set_free (dfa->edests + i); } re_free (dfa->edests); re_free (dfa->eclosures); re_free (dfa->inveclosures); re_free (dfa->nodes); if (dfa->state_table) for (i = 0; i <= dfa->state_hash_mask; ++i) { struct re_state_table_entry *entry = dfa->state_table + i; for (j = 0; j < entry->num; ++j) { re_dfastate_t *state = entry->array[j]; free_state (state); } re_free (entry->array); } re_free (dfa->state_table); #ifdef RE_ENABLE_I18N if (dfa->sb_char != utf8_sb_map) re_free (dfa->sb_char); #endif re_free (dfa->subexp_map); #ifdef DEBUG re_free (dfa->re_str); #endif re_free (dfa); } /* Free dynamically allocated space used by PREG. */ void regfree (regex_t *preg) { re_dfa_t *dfa = preg->buffer; if (BE (dfa != NULL, 1)) { lock_fini (dfa->lock); free_dfa_content (dfa); } preg->buffer = NULL; preg->allocated = 0; re_free (preg->fastmap); preg->fastmap = NULL; re_free (preg->translate); preg->translate = NULL; } #ifdef _LIBC libc_hidden_def (__regfree) weak_alias (__regfree, regfree) #endif /* Entry points compatible with 4.2 BSD regex library. We don't define them unless specifically requested. */ #if defined _REGEX_RE_COMP || defined _LIBC /* BSD has one and only one pattern buffer. */ static struct re_pattern_buffer re_comp_buf; char * # ifdef _LIBC /* Make these definitions weak in libc, so POSIX programs can redefine these names if they don't use our functions, and still use regcomp/regexec above without link errors. */ weak_function # endif re_comp (const char *s) { reg_errcode_t ret; char *fastmap; if (!s) { if (!re_comp_buf.buffer) return gettext ("No previous regular expression"); return 0; } if (re_comp_buf.buffer) { fastmap = re_comp_buf.fastmap; re_comp_buf.fastmap = NULL; __regfree (&re_comp_buf); memset (&re_comp_buf, '\0', sizeof (re_comp_buf)); re_comp_buf.fastmap = fastmap; } if (re_comp_buf.fastmap == NULL) { re_comp_buf.fastmap = re_malloc (char, SBC_MAX); if (re_comp_buf.fastmap == NULL) return (char *) gettext (__re_error_msgid + __re_error_msgid_idx[(int) REG_ESPACE]); } /* Since 're_exec' always passes NULL for the 'regs' argument, we don't need to initialize the pattern buffer fields which affect it. */ /* Match anchors at newlines. */ re_comp_buf.newline_anchor = 1; ret = re_compile_internal (&re_comp_buf, s, strlen (s), re_syntax_options); if (!ret) return NULL; /* Yes, we're discarding 'const' here if !HAVE_LIBINTL. */ return (char *) gettext (__re_error_msgid + __re_error_msgid_idx[(int) ret]); } #ifdef _LIBC libc_freeres_fn (free_mem) { __regfree (&re_comp_buf); } #endif #endif /* _REGEX_RE_COMP */ /* Internal entry point. Compile the regular expression PATTERN, whose length is LENGTH. SYNTAX indicate regular expression's syntax. */ static reg_errcode_t re_compile_internal (regex_t *preg, const char * pattern, size_t length, reg_syntax_t syntax) { reg_errcode_t err = REG_NOERROR; re_dfa_t *dfa; re_string_t regexp; /* Initialize the pattern buffer. */ preg->fastmap_accurate = 0; preg->syntax = syntax; preg->not_bol = preg->not_eol = 0; preg->used = 0; preg->re_nsub = 0; preg->can_be_null = 0; preg->regs_allocated = REGS_UNALLOCATED; /* Initialize the dfa. */ dfa = preg->buffer; if (BE (preg->allocated < sizeof (re_dfa_t), 0)) { /* If zero allocated, but buffer is non-null, try to realloc enough space. This loses if buffer's address is bogus, but that is the user's responsibility. If ->buffer is NULL this is a simple allocation. */ dfa = re_realloc (preg->buffer, re_dfa_t, 1); if (dfa == NULL) return REG_ESPACE; preg->allocated = sizeof (re_dfa_t); preg->buffer = dfa; } preg->used = sizeof (re_dfa_t); err = init_dfa (dfa, length); if (BE (err == REG_NOERROR && lock_init (dfa->lock) != 0, 0)) err = REG_ESPACE; if (BE (err != REG_NOERROR, 0)) { free_dfa_content (dfa); preg->buffer = NULL; preg->allocated = 0; return err; } #ifdef DEBUG /* Note: length+1 will not overflow since it is checked in init_dfa. */ dfa->re_str = re_malloc (char, length + 1); strncpy (dfa->re_str, pattern, length + 1); #endif err = re_string_construct (®exp, pattern, length, preg->translate, (syntax & RE_ICASE) != 0, dfa); if (BE (err != REG_NOERROR, 0)) { re_compile_internal_free_return: free_workarea_compile (preg); re_string_destruct (®exp); lock_fini (dfa->lock); free_dfa_content (dfa); preg->buffer = NULL; preg->allocated = 0; return err; } /* Parse the regular expression, and build a structure tree. */ preg->re_nsub = 0; dfa->str_tree = parse (®exp, preg, syntax, &err); if (BE (dfa->str_tree == NULL, 0)) goto re_compile_internal_free_return; /* Analyze the tree and create the nfa. */ err = analyze (preg); if (BE (err != REG_NOERROR, 0)) goto re_compile_internal_free_return; #ifdef RE_ENABLE_I18N /* If possible, do searching in single byte encoding to speed things up. */ if (dfa->is_utf8 && !(syntax & RE_ICASE) && preg->translate == NULL) optimize_utf8 (dfa); #endif /* Then create the initial state of the dfa. */ err = create_initial_state (dfa); /* Release work areas. */ free_workarea_compile (preg); re_string_destruct (®exp); if (BE (err != REG_NOERROR, 0)) { lock_fini (dfa->lock); free_dfa_content (dfa); preg->buffer = NULL; preg->allocated = 0; } return err; } /* Initialize DFA. We use the length of the regular expression PAT_LEN as the initial length of some arrays. */ static reg_errcode_t init_dfa (re_dfa_t *dfa, size_t pat_len) { __re_size_t table_size; #ifndef _LIBC const char *codeset_name; #endif #ifdef RE_ENABLE_I18N size_t max_i18n_object_size = MAX (sizeof (wchar_t), sizeof (wctype_t)); #else size_t max_i18n_object_size = 0; #endif size_t max_object_size = MAX (sizeof (struct re_state_table_entry), MAX (sizeof (re_token_t), MAX (sizeof (re_node_set), MAX (sizeof (regmatch_t), max_i18n_object_size)))); memset (dfa, '\0', sizeof (re_dfa_t)); /* Force allocation of str_tree_storage the first time. */ dfa->str_tree_storage_idx = BIN_TREE_STORAGE_SIZE; /* Avoid overflows. The extra "/ 2" is for the table_size doubling calculation below, and for similar doubling calculations elsewhere. And it's <= rather than <, because some of the doubling calculations add 1 afterwards. */ if (BE (MIN (IDX_MAX, SIZE_MAX / max_object_size) / 2 <= pat_len, 0)) return REG_ESPACE; dfa->nodes_alloc = pat_len + 1; dfa->nodes = re_malloc (re_token_t, dfa->nodes_alloc); /* table_size = 2 ^ ceil(log pat_len) */ for (table_size = 1; ; table_size <<= 1) if (table_size > pat_len) break; dfa->state_table = calloc (sizeof (struct re_state_table_entry), table_size); dfa->state_hash_mask = table_size - 1; dfa->mb_cur_max = MB_CUR_MAX; #ifdef _LIBC if (dfa->mb_cur_max == 6 && strcmp (_NL_CURRENT (LC_CTYPE, _NL_CTYPE_CODESET_NAME), "UTF-8") == 0) dfa->is_utf8 = 1; dfa->map_notascii = (_NL_CURRENT_WORD (LC_CTYPE, _NL_CTYPE_MAP_TO_NONASCII) != 0); #else codeset_name = nl_langinfo (CODESET); if ((codeset_name[0] == 'U' || codeset_name[0] == 'u') && (codeset_name[1] == 'T' || codeset_name[1] == 't') && (codeset_name[2] == 'F' || codeset_name[2] == 'f') && strcmp (codeset_name + 3 + (codeset_name[3] == '-'), "8") == 0) dfa->is_utf8 = 1; /* We check exhaustively in the loop below if this charset is a superset of ASCII. */ dfa->map_notascii = 0; #endif #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { if (dfa->is_utf8) dfa->sb_char = (re_bitset_ptr_t) utf8_sb_map; else { int i, j, ch; dfa->sb_char = (re_bitset_ptr_t) calloc (sizeof (bitset_t), 1); if (BE (dfa->sb_char == NULL, 0)) return REG_ESPACE; /* Set the bits corresponding to single byte chars. */ for (i = 0, ch = 0; i < BITSET_WORDS; ++i) for (j = 0; j < BITSET_WORD_BITS; ++j, ++ch) { wint_t wch = __btowc (ch); if (wch != WEOF) dfa->sb_char[i] |= (bitset_word_t) 1 << j; # ifndef _LIBC if (isascii (ch) && wch != ch) dfa->map_notascii = 1; # endif } } } #endif if (BE (dfa->nodes == NULL || dfa->state_table == NULL, 0)) return REG_ESPACE; return REG_NOERROR; } /* Initialize WORD_CHAR table, which indicate which character is "word". In this case "word" means that it is the word construction character used by some operators like "\<", "\>", etc. */ static void init_word_char (re_dfa_t *dfa) { int i = 0; int j; int ch = 0; dfa->word_ops_used = 1; if (BE (dfa->map_notascii == 0, 1)) { /* Avoid uint32_t and uint64_t as some non-GCC platforms lack them, an issue when this code is used in Gnulib. */ bitset_word_t bits0 = 0x00000000; bitset_word_t bits1 = 0x03ff0000; bitset_word_t bits2 = 0x87fffffe; bitset_word_t bits3 = 0x07fffffe; if (BITSET_WORD_BITS == 64) { /* Pacify gcc -Woverflow on 32-bit platformns. */ dfa->word_char[0] = bits1 << 31 << 1 | bits0; dfa->word_char[1] = bits3 << 31 << 1 | bits2; i = 2; } else if (BITSET_WORD_BITS == 32) { dfa->word_char[0] = bits0; dfa->word_char[1] = bits1; dfa->word_char[2] = bits2; dfa->word_char[3] = bits3; i = 4; } else goto general_case; ch = 128; if (BE (dfa->is_utf8, 1)) { memset (&dfa->word_char[i], '\0', (SBC_MAX - ch) / 8); return; } } general_case: for (; i < BITSET_WORDS; ++i) for (j = 0; j < BITSET_WORD_BITS; ++j, ++ch) if (isalnum (ch) || ch == '_') dfa->word_char[i] |= (bitset_word_t) 1 << j; } /* Free the work area which are only used while compiling. */ static void free_workarea_compile (regex_t *preg) { re_dfa_t *dfa = preg->buffer; bin_tree_storage_t *storage, *next; for (storage = dfa->str_tree_storage; storage; storage = next) { next = storage->next; re_free (storage); } dfa->str_tree_storage = NULL; dfa->str_tree_storage_idx = BIN_TREE_STORAGE_SIZE; dfa->str_tree = NULL; re_free (dfa->org_indices); dfa->org_indices = NULL; } /* Create initial states for all contexts. */ static reg_errcode_t create_initial_state (re_dfa_t *dfa) { Idx first, i; reg_errcode_t err; re_node_set init_nodes; /* Initial states have the epsilon closure of the node which is the first node of the regular expression. */ first = dfa->str_tree->first->node_idx; dfa->init_node = first; err = re_node_set_init_copy (&init_nodes, dfa->eclosures + first); if (BE (err != REG_NOERROR, 0)) return err; /* The back-references which are in initial states can epsilon transit, since in this case all of the subexpressions can be null. Then we add epsilon closures of the nodes which are the next nodes of the back-references. */ if (dfa->nbackref > 0) for (i = 0; i < init_nodes.nelem; ++i) { Idx node_idx = init_nodes.elems[i]; re_token_type_t type = dfa->nodes[node_idx].type; Idx clexp_idx; if (type != OP_BACK_REF) continue; for (clexp_idx = 0; clexp_idx < init_nodes.nelem; ++clexp_idx) { re_token_t *clexp_node; clexp_node = dfa->nodes + init_nodes.elems[clexp_idx]; if (clexp_node->type == OP_CLOSE_SUBEXP && clexp_node->opr.idx == dfa->nodes[node_idx].opr.idx) break; } if (clexp_idx == init_nodes.nelem) continue; if (type == OP_BACK_REF) { Idx dest_idx = dfa->edests[node_idx].elems[0]; if (!re_node_set_contains (&init_nodes, dest_idx)) { reg_errcode_t merge_err = re_node_set_merge (&init_nodes, dfa->eclosures + dest_idx); if (merge_err != REG_NOERROR) return merge_err; i = 0; } } } /* It must be the first time to invoke acquire_state. */ dfa->init_state = re_acquire_state_context (&err, dfa, &init_nodes, 0); /* We don't check ERR here, since the initial state must not be NULL. */ if (BE (dfa->init_state == NULL, 0)) return err; if (dfa->init_state->has_constraint) { dfa->init_state_word = re_acquire_state_context (&err, dfa, &init_nodes, CONTEXT_WORD); dfa->init_state_nl = re_acquire_state_context (&err, dfa, &init_nodes, CONTEXT_NEWLINE); dfa->init_state_begbuf = re_acquire_state_context (&err, dfa, &init_nodes, CONTEXT_NEWLINE | CONTEXT_BEGBUF); if (BE (dfa->init_state_word == NULL || dfa->init_state_nl == NULL || dfa->init_state_begbuf == NULL, 0)) return err; } else dfa->init_state_word = dfa->init_state_nl = dfa->init_state_begbuf = dfa->init_state; re_node_set_free (&init_nodes); return REG_NOERROR; } #ifdef RE_ENABLE_I18N /* If it is possible to do searching in single byte encoding instead of UTF-8 to speed things up, set dfa->mb_cur_max to 1, clear is_utf8 and change DFA nodes where needed. */ static void optimize_utf8 (re_dfa_t *dfa) { Idx node; int i; bool mb_chars = false; bool has_period = false; for (node = 0; node < dfa->nodes_len; ++node) switch (dfa->nodes[node].type) { case CHARACTER: if (dfa->nodes[node].opr.c >= ASCII_CHARS) mb_chars = true; break; case ANCHOR: switch (dfa->nodes[node].opr.ctx_type) { case LINE_FIRST: case LINE_LAST: case BUF_FIRST: case BUF_LAST: break; default: /* Word anchors etc. cannot be handled. It's okay to test opr.ctx_type since constraints (for all DFA nodes) are created by ORing one or more opr.ctx_type values. */ return; } break; case OP_PERIOD: has_period = true; break; case OP_BACK_REF: case OP_ALT: case END_OF_RE: case OP_DUP_ASTERISK: case OP_OPEN_SUBEXP: case OP_CLOSE_SUBEXP: break; case COMPLEX_BRACKET: return; case SIMPLE_BRACKET: /* Just double check. */ { int rshift = (ASCII_CHARS % BITSET_WORD_BITS == 0 ? 0 : BITSET_WORD_BITS - ASCII_CHARS % BITSET_WORD_BITS); for (i = ASCII_CHARS / BITSET_WORD_BITS; i < BITSET_WORDS; ++i) { if (dfa->nodes[node].opr.sbcset[i] >> rshift != 0) return; rshift = 0; } } break; default: abort (); } if (mb_chars || has_period) for (node = 0; node < dfa->nodes_len; ++node) { if (dfa->nodes[node].type == CHARACTER && dfa->nodes[node].opr.c >= ASCII_CHARS) dfa->nodes[node].mb_partial = 0; else if (dfa->nodes[node].type == OP_PERIOD) dfa->nodes[node].type = OP_UTF8_PERIOD; } /* The search can be in single byte locale. */ dfa->mb_cur_max = 1; dfa->is_utf8 = 0; dfa->has_mb_node = dfa->nbackref > 0 || has_period; } #endif /* Analyze the structure tree, and calculate "first", "next", "edest", "eclosure", and "inveclosure". */ static reg_errcode_t analyze (regex_t *preg) { re_dfa_t *dfa = preg->buffer; reg_errcode_t ret; /* Allocate arrays. */ dfa->nexts = re_malloc (Idx, dfa->nodes_alloc); dfa->org_indices = re_malloc (Idx, dfa->nodes_alloc); dfa->edests = re_malloc (re_node_set, dfa->nodes_alloc); dfa->eclosures = re_malloc (re_node_set, dfa->nodes_alloc); if (BE (dfa->nexts == NULL || dfa->org_indices == NULL || dfa->edests == NULL || dfa->eclosures == NULL, 0)) return REG_ESPACE; dfa->subexp_map = re_malloc (Idx, preg->re_nsub); if (dfa->subexp_map != NULL) { Idx i; for (i = 0; i < preg->re_nsub; i++) dfa->subexp_map[i] = i; preorder (dfa->str_tree, optimize_subexps, dfa); for (i = 0; i < preg->re_nsub; i++) if (dfa->subexp_map[i] != i) break; if (i == preg->re_nsub) { re_free (dfa->subexp_map); dfa->subexp_map = NULL; } } ret = postorder (dfa->str_tree, lower_subexps, preg); if (BE (ret != REG_NOERROR, 0)) return ret; ret = postorder (dfa->str_tree, calc_first, dfa); if (BE (ret != REG_NOERROR, 0)) return ret; preorder (dfa->str_tree, calc_next, dfa); ret = preorder (dfa->str_tree, link_nfa_nodes, dfa); if (BE (ret != REG_NOERROR, 0)) return ret; ret = calc_eclosure (dfa); if (BE (ret != REG_NOERROR, 0)) return ret; /* We only need this during the prune_impossible_nodes pass in regexec.c; skip it if p_i_n will not run, as calc_inveclosure can be quadratic. */ if ((!preg->no_sub && preg->re_nsub > 0 && dfa->has_plural_match) || dfa->nbackref) { dfa->inveclosures = re_malloc (re_node_set, dfa->nodes_len); if (BE (dfa->inveclosures == NULL, 0)) return REG_ESPACE; ret = calc_inveclosure (dfa); } return ret; } /* Our parse trees are very unbalanced, so we cannot use a stack to implement parse tree visits. Instead, we use parent pointers and some hairy code in these two functions. */ static reg_errcode_t postorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra) { bin_tree_t *node, *prev; for (node = root; ; ) { /* Descend down the tree, preferably to the left (or to the right if that's the only child). */ while (node->left || node->right) if (node->left) node = node->left; else node = node->right; do { reg_errcode_t err = fn (extra, node); if (BE (err != REG_NOERROR, 0)) return err; if (node->parent == NULL) return REG_NOERROR; prev = node; node = node->parent; } /* Go up while we have a node that is reached from the right. */ while (node->right == prev || node->right == NULL); node = node->right; } } static reg_errcode_t preorder (bin_tree_t *root, reg_errcode_t (fn (void *, bin_tree_t *)), void *extra) { bin_tree_t *node; for (node = root; ; ) { reg_errcode_t err = fn (extra, node); if (BE (err != REG_NOERROR, 0)) return err; /* Go to the left node, or up and to the right. */ if (node->left) node = node->left; else { bin_tree_t *prev = NULL; while (node->right == prev || node->right == NULL) { prev = node; node = node->parent; if (!node) return REG_NOERROR; } node = node->right; } } } /* Optimization pass: if a SUBEXP is entirely contained, strip it and tell re_search_internal to map the inner one's opr.idx to this one's. Adjust backreferences as well. Requires a preorder visit. */ static reg_errcode_t optimize_subexps (void *extra, bin_tree_t *node) { re_dfa_t *dfa = (re_dfa_t *) extra; if (node->token.type == OP_BACK_REF && dfa->subexp_map) { int idx = node->token.opr.idx; node->token.opr.idx = dfa->subexp_map[idx]; dfa->used_bkref_map |= 1 << node->token.opr.idx; } else if (node->token.type == SUBEXP && node->left && node->left->token.type == SUBEXP) { Idx other_idx = node->left->token.opr.idx; node->left = node->left->left; if (node->left) node->left->parent = node; dfa->subexp_map[other_idx] = dfa->subexp_map[node->token.opr.idx]; if (other_idx < BITSET_WORD_BITS) dfa->used_bkref_map &= ~((bitset_word_t) 1 << other_idx); } return REG_NOERROR; } /* Lowering pass: Turn each SUBEXP node into the appropriate concatenation of OP_OPEN_SUBEXP, the body of the SUBEXP (if any) and OP_CLOSE_SUBEXP. */ static reg_errcode_t lower_subexps (void *extra, bin_tree_t *node) { regex_t *preg = (regex_t *) extra; reg_errcode_t err = REG_NOERROR; if (node->left && node->left->token.type == SUBEXP) { node->left = lower_subexp (&err, preg, node->left); if (node->left) node->left->parent = node; } if (node->right && node->right->token.type == SUBEXP) { node->right = lower_subexp (&err, preg, node->right); if (node->right) node->right->parent = node; } return err; } static bin_tree_t * lower_subexp (reg_errcode_t *err, regex_t *preg, bin_tree_t *node) { re_dfa_t *dfa = preg->buffer; bin_tree_t *body = node->left; bin_tree_t *op, *cls, *tree1, *tree; if (preg->no_sub /* We do not optimize empty subexpressions, because otherwise we may have bad CONCAT nodes with NULL children. This is obviously not very common, so we do not lose much. An example that triggers this case is the sed "script" /\(\)/x. */ && node->left != NULL && (node->token.opr.idx >= BITSET_WORD_BITS || !(dfa->used_bkref_map & ((bitset_word_t) 1 << node->token.opr.idx)))) return node->left; /* Convert the SUBEXP node to the concatenation of an OP_OPEN_SUBEXP, the contents, and an OP_CLOSE_SUBEXP. */ op = create_tree (dfa, NULL, NULL, OP_OPEN_SUBEXP); cls = create_tree (dfa, NULL, NULL, OP_CLOSE_SUBEXP); tree1 = body ? create_tree (dfa, body, cls, CONCAT) : cls; tree = create_tree (dfa, op, tree1, CONCAT); if (BE (tree == NULL || tree1 == NULL || op == NULL || cls == NULL, 0)) { *err = REG_ESPACE; return NULL; } op->token.opr.idx = cls->token.opr.idx = node->token.opr.idx; op->token.opt_subexp = cls->token.opt_subexp = node->token.opt_subexp; return tree; } /* Pass 1 in building the NFA: compute FIRST and create unlinked automaton nodes. Requires a postorder visit. */ static reg_errcode_t calc_first (void *extra, bin_tree_t *node) { re_dfa_t *dfa = (re_dfa_t *) extra; if (node->token.type == CONCAT) { node->first = node->left->first; node->node_idx = node->left->node_idx; } else { node->first = node; node->node_idx = re_dfa_add_node (dfa, node->token); if (BE (node->node_idx == -1, 0)) return REG_ESPACE; if (node->token.type == ANCHOR) dfa->nodes[node->node_idx].constraint = node->token.opr.ctx_type; } return REG_NOERROR; } /* Pass 2: compute NEXT on the tree. Preorder visit. */ static reg_errcode_t calc_next (void *extra, bin_tree_t *node) { switch (node->token.type) { case OP_DUP_ASTERISK: node->left->next = node; break; case CONCAT: node->left->next = node->right->first; node->right->next = node->next; break; default: if (node->left) node->left->next = node->next; if (node->right) node->right->next = node->next; break; } return REG_NOERROR; } /* Pass 3: link all DFA nodes to their NEXT node (any order will do). */ static reg_errcode_t link_nfa_nodes (void *extra, bin_tree_t *node) { re_dfa_t *dfa = (re_dfa_t *) extra; Idx idx = node->node_idx; reg_errcode_t err = REG_NOERROR; switch (node->token.type) { case CONCAT: break; case END_OF_RE: assert (node->next == NULL); break; case OP_DUP_ASTERISK: case OP_ALT: { Idx left, right; dfa->has_plural_match = 1; if (node->left != NULL) left = node->left->first->node_idx; else left = node->next->node_idx; if (node->right != NULL) right = node->right->first->node_idx; else right = node->next->node_idx; assert (left > -1); assert (right > -1); err = re_node_set_init_2 (dfa->edests + idx, left, right); } break; case ANCHOR: case OP_OPEN_SUBEXP: case OP_CLOSE_SUBEXP: err = re_node_set_init_1 (dfa->edests + idx, node->next->node_idx); break; case OP_BACK_REF: dfa->nexts[idx] = node->next->node_idx; if (node->token.type == OP_BACK_REF) err = re_node_set_init_1 (dfa->edests + idx, dfa->nexts[idx]); break; default: assert (!IS_EPSILON_NODE (node->token.type)); dfa->nexts[idx] = node->next->node_idx; break; } return err; } /* Duplicate the epsilon closure of the node ROOT_NODE. Note that duplicated nodes have constraint INIT_CONSTRAINT in addition to their own constraint. */ static reg_errcode_t duplicate_node_closure (re_dfa_t *dfa, Idx top_org_node, Idx top_clone_node, Idx root_node, unsigned int init_constraint) { Idx org_node, clone_node; bool ok; unsigned int constraint = init_constraint; for (org_node = top_org_node, clone_node = top_clone_node;;) { Idx org_dest, clone_dest; if (dfa->nodes[org_node].type == OP_BACK_REF) { /* If the back reference epsilon-transit, its destination must also have the constraint. Then duplicate the epsilon closure of the destination of the back reference, and store it in edests of the back reference. */ org_dest = dfa->nexts[org_node]; re_node_set_empty (dfa->edests + clone_node); clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; dfa->nexts[clone_node] = dfa->nexts[org_node]; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } else if (dfa->edests[org_node].nelem == 0) { /* In case of the node can't epsilon-transit, don't duplicate the destination and store the original destination as the destination of the node. */ dfa->nexts[clone_node] = dfa->nexts[org_node]; break; } else if (dfa->edests[org_node].nelem == 1) { /* In case of the node can epsilon-transit, and it has only one destination. */ org_dest = dfa->edests[org_node].elems[0]; re_node_set_empty (dfa->edests + clone_node); /* If the node is root_node itself, it means the epsilon closure has a loop. Then tie it to the destination of the root_node. */ if (org_node == root_node && clone_node != org_node) { ok = re_node_set_insert (dfa->edests + clone_node, org_dest); if (BE (! ok, 0)) return REG_ESPACE; break; } /* In case the node has another constraint, append it. */ constraint |= dfa->nodes[org_node].constraint; clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } else /* dfa->edests[org_node].nelem == 2 */ { /* In case of the node can epsilon-transit, and it has two destinations. In the bin_tree_t and DFA, that's '|' and '*'. */ org_dest = dfa->edests[org_node].elems[0]; re_node_set_empty (dfa->edests + clone_node); /* Search for a duplicated node which satisfies the constraint. */ clone_dest = search_duplicated_node (dfa, org_dest, constraint); if (clone_dest == -1) { /* There is no such duplicated node, create a new one. */ reg_errcode_t err; clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; err = duplicate_node_closure (dfa, org_dest, clone_dest, root_node, constraint); if (BE (err != REG_NOERROR, 0)) return err; } else { /* There is a duplicated node which satisfies the constraint, use it to avoid infinite loop. */ ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } org_dest = dfa->edests[org_node].elems[1]; clone_dest = duplicate_node (dfa, org_dest, constraint); if (BE (clone_dest == -1, 0)) return REG_ESPACE; ok = re_node_set_insert (dfa->edests + clone_node, clone_dest); if (BE (! ok, 0)) return REG_ESPACE; } org_node = org_dest; clone_node = clone_dest; } return REG_NOERROR; } /* Search for a node which is duplicated from the node ORG_NODE, and satisfies the constraint CONSTRAINT. */ static Idx search_duplicated_node (const re_dfa_t *dfa, Idx org_node, unsigned int constraint) { Idx idx; for (idx = dfa->nodes_len - 1; dfa->nodes[idx].duplicated && idx > 0; --idx) { if (org_node == dfa->org_indices[idx] && constraint == dfa->nodes[idx].constraint) return idx; /* Found. */ } return -1; /* Not found. */ } /* Duplicate the node whose index is ORG_IDX and set the constraint CONSTRAINT. Return the index of the new node, or -1 if insufficient storage is available. */ static Idx duplicate_node (re_dfa_t *dfa, Idx org_idx, unsigned int constraint) { Idx dup_idx = re_dfa_add_node (dfa, dfa->nodes[org_idx]); if (BE (dup_idx != -1, 1)) { dfa->nodes[dup_idx].constraint = constraint; dfa->nodes[dup_idx].constraint |= dfa->nodes[org_idx].constraint; dfa->nodes[dup_idx].duplicated = 1; /* Store the index of the original node. */ dfa->org_indices[dup_idx] = org_idx; } return dup_idx; } static reg_errcode_t calc_inveclosure (re_dfa_t *dfa) { Idx src, idx; bool ok; for (idx = 0; idx < dfa->nodes_len; ++idx) re_node_set_init_empty (dfa->inveclosures + idx); for (src = 0; src < dfa->nodes_len; ++src) { Idx *elems = dfa->eclosures[src].elems; for (idx = 0; idx < dfa->eclosures[src].nelem; ++idx) { ok = re_node_set_insert_last (dfa->inveclosures + elems[idx], src); if (BE (! ok, 0)) return REG_ESPACE; } } return REG_NOERROR; } /* Calculate "eclosure" for all the node in DFA. */ static reg_errcode_t calc_eclosure (re_dfa_t *dfa) { Idx node_idx; bool incomplete; #ifdef DEBUG assert (dfa->nodes_len > 0); #endif incomplete = false; /* For each nodes, calculate epsilon closure. */ for (node_idx = 0; ; ++node_idx) { reg_errcode_t err; re_node_set eclosure_elem; if (node_idx == dfa->nodes_len) { if (!incomplete) break; incomplete = false; node_idx = 0; } #ifdef DEBUG assert (dfa->eclosures[node_idx].nelem != -1); #endif /* If we have already calculated, skip it. */ if (dfa->eclosures[node_idx].nelem != 0) continue; /* Calculate epsilon closure of 'node_idx'. */ err = calc_eclosure_iter (&eclosure_elem, dfa, node_idx, true); if (BE (err != REG_NOERROR, 0)) return err; if (dfa->eclosures[node_idx].nelem == 0) { incomplete = true; re_node_set_free (&eclosure_elem); } } return REG_NOERROR; } /* Calculate epsilon closure of NODE. */ static reg_errcode_t calc_eclosure_iter (re_node_set *new_set, re_dfa_t *dfa, Idx node, bool root) { reg_errcode_t err; Idx i; re_node_set eclosure; bool ok; bool incomplete = false; err = re_node_set_alloc (&eclosure, dfa->edests[node].nelem + 1); if (BE (err != REG_NOERROR, 0)) return err; /* This indicates that we are calculating this node now. We reference this value to avoid infinite loop. */ dfa->eclosures[node].nelem = -1; /* If the current node has constraints, duplicate all nodes since they must inherit the constraints. */ if (dfa->nodes[node].constraint && dfa->edests[node].nelem && !dfa->nodes[dfa->edests[node].elems[0]].duplicated) { err = duplicate_node_closure (dfa, node, node, node, dfa->nodes[node].constraint); if (BE (err != REG_NOERROR, 0)) return err; } /* Expand each epsilon destination nodes. */ if (IS_EPSILON_NODE(dfa->nodes[node].type)) for (i = 0; i < dfa->edests[node].nelem; ++i) { re_node_set eclosure_elem; Idx edest = dfa->edests[node].elems[i]; /* If calculating the epsilon closure of 'edest' is in progress, return intermediate result. */ if (dfa->eclosures[edest].nelem == -1) { incomplete = true; continue; } /* If we haven't calculated the epsilon closure of 'edest' yet, calculate now. Otherwise use calculated epsilon closure. */ if (dfa->eclosures[edest].nelem == 0) { err = calc_eclosure_iter (&eclosure_elem, dfa, edest, false); if (BE (err != REG_NOERROR, 0)) return err; } else eclosure_elem = dfa->eclosures[edest]; /* Merge the epsilon closure of 'edest'. */ err = re_node_set_merge (&eclosure, &eclosure_elem); if (BE (err != REG_NOERROR, 0)) return err; /* If the epsilon closure of 'edest' is incomplete, the epsilon closure of this node is also incomplete. */ if (dfa->eclosures[edest].nelem == 0) { incomplete = true; re_node_set_free (&eclosure_elem); } } /* An epsilon closure includes itself. */ ok = re_node_set_insert (&eclosure, node); if (BE (! ok, 0)) return REG_ESPACE; if (incomplete && !root) dfa->eclosures[node].nelem = 0; else dfa->eclosures[node] = eclosure; *new_set = eclosure; return REG_NOERROR; } /* Functions for token which are used in the parser. */ /* Fetch a token from INPUT. We must not use this function inside bracket expressions. */ static void fetch_token (re_token_t *result, re_string_t *input, reg_syntax_t syntax) { re_string_skip_bytes (input, peek_token (result, input, syntax)); } /* Peek a token from INPUT, and return the length of the token. We must not use this function inside bracket expressions. */ static int peek_token (re_token_t *token, re_string_t *input, reg_syntax_t syntax) { unsigned char c; if (re_string_eoi (input)) { token->type = END_OF_RE; return 0; } c = re_string_peek_byte (input, 0); token->opr.c = c; token->word_char = 0; #ifdef RE_ENABLE_I18N token->mb_partial = 0; if (input->mb_cur_max > 1 && !re_string_first_byte (input, re_string_cur_idx (input))) { token->type = CHARACTER; token->mb_partial = 1; return 1; } #endif if (c == '\\') { unsigned char c2; if (re_string_cur_idx (input) + 1 >= re_string_length (input)) { token->type = BACK_SLASH; return 1; } c2 = re_string_peek_byte_case (input, 1); token->opr.c = c2; token->type = CHARACTER; #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1) { wint_t wc = re_string_wchar_at (input, re_string_cur_idx (input) + 1); token->word_char = IS_WIDE_WORD_CHAR (wc) != 0; } else #endif token->word_char = IS_WORD_CHAR (c2) != 0; switch (c2) { case '|': if (!(syntax & RE_LIMITED_OPS) && !(syntax & RE_NO_BK_VBAR)) token->type = OP_ALT; break; case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': if (!(syntax & RE_NO_BK_REFS)) { token->type = OP_BACK_REF; token->opr.idx = c2 - '1'; } break; case '<': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = WORD_FIRST; } break; case '>': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = WORD_LAST; } break; case 'b': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = WORD_DELIM; } break; case 'B': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = NOT_WORD_DELIM; } break; case 'w': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_WORD; break; case 'W': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_NOTWORD; break; case 's': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_SPACE; break; case 'S': if (!(syntax & RE_NO_GNU_OPS)) token->type = OP_NOTSPACE; break; case '`': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = BUF_FIRST; } break; case '\'': if (!(syntax & RE_NO_GNU_OPS)) { token->type = ANCHOR; token->opr.ctx_type = BUF_LAST; } break; case '(': if (!(syntax & RE_NO_BK_PARENS)) token->type = OP_OPEN_SUBEXP; break; case ')': if (!(syntax & RE_NO_BK_PARENS)) token->type = OP_CLOSE_SUBEXP; break; case '+': if (!(syntax & RE_LIMITED_OPS) && (syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_PLUS; break; case '?': if (!(syntax & RE_LIMITED_OPS) && (syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_QUESTION; break; case '{': if ((syntax & RE_INTERVALS) && (!(syntax & RE_NO_BK_BRACES))) token->type = OP_OPEN_DUP_NUM; break; case '}': if ((syntax & RE_INTERVALS) && (!(syntax & RE_NO_BK_BRACES))) token->type = OP_CLOSE_DUP_NUM; break; default: break; } return 2; } token->type = CHARACTER; #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1) { wint_t wc = re_string_wchar_at (input, re_string_cur_idx (input)); token->word_char = IS_WIDE_WORD_CHAR (wc) != 0; } else #endif token->word_char = IS_WORD_CHAR (token->opr.c); switch (c) { case '\n': if (syntax & RE_NEWLINE_ALT) token->type = OP_ALT; break; case '|': if (!(syntax & RE_LIMITED_OPS) && (syntax & RE_NO_BK_VBAR)) token->type = OP_ALT; break; case '*': token->type = OP_DUP_ASTERISK; break; case '+': if (!(syntax & RE_LIMITED_OPS) && !(syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_PLUS; break; case '?': if (!(syntax & RE_LIMITED_OPS) && !(syntax & RE_BK_PLUS_QM)) token->type = OP_DUP_QUESTION; break; case '{': if ((syntax & RE_INTERVALS) && (syntax & RE_NO_BK_BRACES)) token->type = OP_OPEN_DUP_NUM; break; case '}': if ((syntax & RE_INTERVALS) && (syntax & RE_NO_BK_BRACES)) token->type = OP_CLOSE_DUP_NUM; break; case '(': if (syntax & RE_NO_BK_PARENS) token->type = OP_OPEN_SUBEXP; break; case ')': if (syntax & RE_NO_BK_PARENS) token->type = OP_CLOSE_SUBEXP; break; case '[': token->type = OP_OPEN_BRACKET; break; case '.': token->type = OP_PERIOD; break; case '^': if (!(syntax & (RE_CONTEXT_INDEP_ANCHORS | RE_CARET_ANCHORS_HERE)) && re_string_cur_idx (input) != 0) { char prev = re_string_peek_byte (input, -1); if (!(syntax & RE_NEWLINE_ALT) || prev != '\n') break; } token->type = ANCHOR; token->opr.ctx_type = LINE_FIRST; break; case '$': if (!(syntax & RE_CONTEXT_INDEP_ANCHORS) && re_string_cur_idx (input) + 1 != re_string_length (input)) { re_token_t next; re_string_skip_bytes (input, 1); peek_token (&next, input, syntax); re_string_skip_bytes (input, -1); if (next.type != OP_ALT && next.type != OP_CLOSE_SUBEXP) break; } token->type = ANCHOR; token->opr.ctx_type = LINE_LAST; break; default: break; } return 1; } /* Peek a token from INPUT, and return the length of the token. We must not use this function out of bracket expressions. */ static int peek_token_bracket (re_token_t *token, re_string_t *input, reg_syntax_t syntax) { unsigned char c; if (re_string_eoi (input)) { token->type = END_OF_RE; return 0; } c = re_string_peek_byte (input, 0); token->opr.c = c; #ifdef RE_ENABLE_I18N if (input->mb_cur_max > 1 && !re_string_first_byte (input, re_string_cur_idx (input))) { token->type = CHARACTER; return 1; } #endif /* RE_ENABLE_I18N */ if (c == '\\' && (syntax & RE_BACKSLASH_ESCAPE_IN_LISTS) && re_string_cur_idx (input) + 1 < re_string_length (input)) { /* In this case, '\' escape a character. */ unsigned char c2; re_string_skip_bytes (input, 1); c2 = re_string_peek_byte (input, 0); token->opr.c = c2; token->type = CHARACTER; return 1; } if (c == '[') /* '[' is a special char in a bracket exps. */ { unsigned char c2; int token_len; if (re_string_cur_idx (input) + 1 < re_string_length (input)) c2 = re_string_peek_byte (input, 1); else c2 = 0; token->opr.c = c2; token_len = 2; switch (c2) { case '.': token->type = OP_OPEN_COLL_ELEM; break; case '=': token->type = OP_OPEN_EQUIV_CLASS; break; case ':': if (syntax & RE_CHAR_CLASSES) { token->type = OP_OPEN_CHAR_CLASS; break; } FALLTHROUGH; default: token->type = CHARACTER; token->opr.c = c; token_len = 1; break; } return token_len; } switch (c) { case '-': token->type = OP_CHARSET_RANGE; break; case ']': token->type = OP_CLOSE_BRACKET; break; case '^': token->type = OP_NON_MATCH_LIST; break; default: token->type = CHARACTER; } return 1; } /* Functions for parser. */ /* Entry point of the parser. Parse the regular expression REGEXP and return the structure tree. If an error occurs, ERR is set by error code, and return NULL. This function build the following tree, from regular expression : CAT / \ / \ EOR CAT means concatenation. EOR means end of regular expression. */ static bin_tree_t * parse (re_string_t *regexp, regex_t *preg, reg_syntax_t syntax, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree, *eor, *root; re_token_t current_token; dfa->syntax = syntax; fetch_token (¤t_token, regexp, syntax | RE_CARET_ANCHORS_HERE); tree = parse_reg_exp (regexp, preg, ¤t_token, syntax, 0, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; eor = create_tree (dfa, NULL, NULL, END_OF_RE); if (tree != NULL) root = create_tree (dfa, tree, eor, CONCAT); else root = eor; if (BE (eor == NULL || root == NULL, 0)) { *err = REG_ESPACE; return NULL; } return root; } /* This function build the following tree, from regular expression |: ALT / \ / \ ALT means alternative, which represents the operator '|'. */ static bin_tree_t * parse_reg_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree, *branch = NULL; bitset_word_t initial_bkref_map = dfa->completed_bkref_map; tree = parse_branch (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; while (token->type == OP_ALT) { fetch_token (token, regexp, syntax | RE_CARET_ANCHORS_HERE); if (token->type != OP_ALT && token->type != END_OF_RE && (nest == 0 || token->type != OP_CLOSE_SUBEXP)) { bitset_word_t accumulated_bkref_map = dfa->completed_bkref_map; dfa->completed_bkref_map = initial_bkref_map; branch = parse_branch (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && branch == NULL, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); return NULL; } dfa->completed_bkref_map |= accumulated_bkref_map; } else branch = NULL; tree = create_tree (dfa, tree, branch, OP_ALT); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } return tree; } /* This function build the following tree, from regular expression : CAT / \ / \ CAT means concatenation. */ static bin_tree_t * parse_branch (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { bin_tree_t *tree, *expr; re_dfa_t *dfa = preg->buffer; tree = parse_expression (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; while (token->type != OP_ALT && token->type != END_OF_RE && (nest == 0 || token->type != OP_CLOSE_SUBEXP)) { expr = parse_expression (regexp, preg, token, syntax, nest, err); if (BE (*err != REG_NOERROR && expr == NULL, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); return NULL; } if (tree != NULL && expr != NULL) { bin_tree_t *newtree = create_tree (dfa, tree, expr, CONCAT); if (newtree == NULL) { postorder (expr, free_tree, NULL); postorder (tree, free_tree, NULL); *err = REG_ESPACE; return NULL; } tree = newtree; } else if (tree == NULL) tree = expr; /* Otherwise expr == NULL, we don't need to create new tree. */ } return tree; } /* This function build the following tree, from regular expression a*: * | a */ static bin_tree_t * parse_expression (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree; switch (token->type) { case CHARACTER: tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { while (!re_string_eoi (regexp) && !re_string_first_byte (regexp, re_string_cur_idx (regexp))) { bin_tree_t *mbc_remain; fetch_token (token, regexp, syntax); mbc_remain = create_token_tree (dfa, NULL, NULL, token); tree = create_tree (dfa, tree, mbc_remain, CONCAT); if (BE (mbc_remain == NULL || tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } } #endif break; case OP_OPEN_SUBEXP: tree = parse_sub_exp (regexp, preg, token, syntax, nest + 1, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_OPEN_BRACKET: tree = parse_bracket_exp (regexp, dfa, token, syntax, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_BACK_REF: if (!BE (dfa->completed_bkref_map & (1 << token->opr.idx), 1)) { *err = REG_ESUBREG; return NULL; } dfa->used_bkref_map |= 1 << token->opr.idx; tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } ++dfa->nbackref; dfa->has_mb_node = 1; break; case OP_OPEN_DUP_NUM: if (syntax & RE_CONTEXT_INVALID_DUP) { *err = REG_BADRPT; return NULL; } FALLTHROUGH; case OP_DUP_ASTERISK: case OP_DUP_PLUS: case OP_DUP_QUESTION: if (syntax & RE_CONTEXT_INVALID_OPS) { *err = REG_BADRPT; return NULL; } else if (syntax & RE_CONTEXT_INDEP_OPS) { fetch_token (token, regexp, syntax); return parse_expression (regexp, preg, token, syntax, nest, err); } FALLTHROUGH; case OP_CLOSE_SUBEXP: if ((token->type == OP_CLOSE_SUBEXP) && !(syntax & RE_UNMATCHED_RIGHT_PAREN_ORD)) { *err = REG_ERPAREN; return NULL; } FALLTHROUGH; case OP_CLOSE_DUP_NUM: /* We treat it as a normal character. */ /* Then we can these characters as normal characters. */ token->type = CHARACTER; /* mb_partial and word_char bits should be initialized already by peek_token. */ tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } break; case ANCHOR: if ((token->opr.ctx_type & (WORD_DELIM | NOT_WORD_DELIM | WORD_FIRST | WORD_LAST)) && dfa->word_ops_used == 0) init_word_char (dfa); if (token->opr.ctx_type == WORD_DELIM || token->opr.ctx_type == NOT_WORD_DELIM) { bin_tree_t *tree_first, *tree_last; if (token->opr.ctx_type == WORD_DELIM) { token->opr.ctx_type = WORD_FIRST; tree_first = create_token_tree (dfa, NULL, NULL, token); token->opr.ctx_type = WORD_LAST; } else { token->opr.ctx_type = INSIDE_WORD; tree_first = create_token_tree (dfa, NULL, NULL, token); token->opr.ctx_type = INSIDE_NOTWORD; } tree_last = create_token_tree (dfa, NULL, NULL, token); tree = create_tree (dfa, tree_first, tree_last, OP_ALT); if (BE (tree_first == NULL || tree_last == NULL || tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } else { tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } } /* We must return here, since ANCHORs can't be followed by repetition operators. eg. RE"^*" is invalid or "", it must not be "". */ fetch_token (token, regexp, syntax); return tree; case OP_PERIOD: tree = create_token_tree (dfa, NULL, NULL, token); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } if (dfa->mb_cur_max > 1) dfa->has_mb_node = 1; break; case OP_WORD: case OP_NOTWORD: tree = build_charclass_op (dfa, regexp->trans, "alnum", "_", token->type == OP_NOTWORD, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_SPACE: case OP_NOTSPACE: tree = build_charclass_op (dfa, regexp->trans, "space", "", token->type == OP_NOTSPACE, err); if (BE (*err != REG_NOERROR && tree == NULL, 0)) return NULL; break; case OP_ALT: case END_OF_RE: return NULL; case BACK_SLASH: *err = REG_EESCAPE; return NULL; default: /* Must not happen? */ #ifdef DEBUG assert (0); #endif return NULL; } fetch_token (token, regexp, syntax); while (token->type == OP_DUP_ASTERISK || token->type == OP_DUP_PLUS || token->type == OP_DUP_QUESTION || token->type == OP_OPEN_DUP_NUM) { bin_tree_t *dup_tree = parse_dup_op (tree, regexp, dfa, token, syntax, err); if (BE (*err != REG_NOERROR && dup_tree == NULL, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); return NULL; } tree = dup_tree; /* In BRE consecutive duplications are not allowed. */ if ((syntax & RE_CONTEXT_INVALID_DUP) && (token->type == OP_DUP_ASTERISK || token->type == OP_OPEN_DUP_NUM)) { if (tree != NULL) postorder (tree, free_tree, NULL); *err = REG_BADRPT; return NULL; } } return tree; } /* This function build the following tree, from regular expression (): SUBEXP | */ static bin_tree_t * parse_sub_exp (re_string_t *regexp, regex_t *preg, re_token_t *token, reg_syntax_t syntax, Idx nest, reg_errcode_t *err) { re_dfa_t *dfa = preg->buffer; bin_tree_t *tree; size_t cur_nsub; cur_nsub = preg->re_nsub++; fetch_token (token, regexp, syntax | RE_CARET_ANCHORS_HERE); /* The subexpression may be a null string. */ if (token->type == OP_CLOSE_SUBEXP) tree = NULL; else { tree = parse_reg_exp (regexp, preg, token, syntax, nest, err); if (BE (*err == REG_NOERROR && token->type != OP_CLOSE_SUBEXP, 0)) { if (tree != NULL) postorder (tree, free_tree, NULL); *err = REG_EPAREN; } if (BE (*err != REG_NOERROR, 0)) return NULL; } if (cur_nsub <= '9' - '1') dfa->completed_bkref_map |= 1 << cur_nsub; tree = create_tree (dfa, tree, NULL, SUBEXP); if (BE (tree == NULL, 0)) { *err = REG_ESPACE; return NULL; } tree->token.opr.idx = cur_nsub; return tree; } /* This function parse repetition operators like "*", "+", "{1,3}" etc. */ static bin_tree_t * parse_dup_op (bin_tree_t *elem, re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err) { bin_tree_t *tree = NULL, *old_tree = NULL; Idx i, start, end, start_idx = re_string_cur_idx (regexp); re_token_t start_token = *token; if (token->type == OP_OPEN_DUP_NUM) { end = 0; start = fetch_number (regexp, token, syntax); if (start == -1) { if (token->type == CHARACTER && token->opr.c == ',') start = 0; /* We treat "{,m}" as "{0,m}". */ else { *err = REG_BADBR; /* {} is invalid. */ return NULL; } } if (BE (start != -2, 1)) { /* We treat "{n}" as "{n,n}". */ end = ((token->type == OP_CLOSE_DUP_NUM) ? start : ((token->type == CHARACTER && token->opr.c == ',') ? fetch_number (regexp, token, syntax) : -2)); } if (BE (start == -2 || end == -2, 0)) { /* Invalid sequence. */ if (BE (!(syntax & RE_INVALID_INTERVAL_ORD), 0)) { if (token->type == END_OF_RE) *err = REG_EBRACE; else *err = REG_BADBR; return NULL; } /* If the syntax bit is set, rollback. */ re_string_set_index (regexp, start_idx); *token = start_token; token->type = CHARACTER; /* mb_partial and word_char bits should be already initialized by peek_token. */ return elem; } if (BE ((end != -1 && start > end) || token->type != OP_CLOSE_DUP_NUM, 0)) { /* First number greater than second. */ *err = REG_BADBR; return NULL; } if (BE (RE_DUP_MAX < (end == -1 ? start : end), 0)) { *err = REG_ESIZE; return NULL; } } else { start = (token->type == OP_DUP_PLUS) ? 1 : 0; end = (token->type == OP_DUP_QUESTION) ? 1 : -1; } fetch_token (token, regexp, syntax); if (BE (elem == NULL, 0)) return NULL; if (BE (start == 0 && end == 0, 0)) { postorder (elem, free_tree, NULL); return NULL; } /* Extract "{n,m}" to "...{0,}". */ if (BE (start > 0, 0)) { tree = elem; for (i = 2; i <= start; ++i) { elem = duplicate_tree (elem, dfa); tree = create_tree (dfa, tree, elem, CONCAT); if (BE (elem == NULL || tree == NULL, 0)) goto parse_dup_op_espace; } if (start == end) return tree; /* Duplicate ELEM before it is marked optional. */ elem = duplicate_tree (elem, dfa); if (BE (elem == NULL, 0)) goto parse_dup_op_espace; old_tree = tree; } else old_tree = NULL; if (elem->token.type == SUBEXP) { uintptr_t subidx = elem->token.opr.idx; postorder (elem, mark_opt_subexp, (void *) subidx); } tree = create_tree (dfa, elem, NULL, (end == -1 ? OP_DUP_ASTERISK : OP_ALT)); if (BE (tree == NULL, 0)) goto parse_dup_op_espace; /* From gnulib's "intprops.h": True if the arithmetic type T is signed. */ #define TYPE_SIGNED(t) (! ((t) 0 < (t) -1)) /* This loop is actually executed only when end != -1, to rewrite {0,n} as ((...?)?)?... We have already created the start+1-th copy. */ if (TYPE_SIGNED (Idx) || end != -1) for (i = start + 2; i <= end; ++i) { elem = duplicate_tree (elem, dfa); tree = create_tree (dfa, tree, elem, CONCAT); if (BE (elem == NULL || tree == NULL, 0)) goto parse_dup_op_espace; tree = create_tree (dfa, tree, NULL, OP_ALT); if (BE (tree == NULL, 0)) goto parse_dup_op_espace; } if (old_tree) tree = create_tree (dfa, old_tree, tree, CONCAT); return tree; parse_dup_op_espace: *err = REG_ESPACE; return NULL; } /* Size of the names for collating symbol/equivalence_class/character_class. I'm not sure, but maybe enough. */ #define BRACKET_NAME_BUF_SIZE 32 #ifndef _LIBC # ifdef RE_ENABLE_I18N /* Convert the byte B to the corresponding wide character. In a unibyte locale, treat B as itself if it is an encoding error. In a multibyte locale, return WEOF if B is an encoding error. */ static wint_t parse_byte (unsigned char b, re_charset_t *mbcset) { wint_t wc = __btowc (b); return wc == WEOF && !mbcset ? b : wc; } #endif /* Local function for parse_bracket_exp only used in case of NOT _LIBC. Build the range expression which starts from START_ELEM, and ends at END_ELEM. The result are written to MBCSET and SBCSET. RANGE_ALLOC is the allocated size of mbcset->range_starts, and mbcset->range_ends, is a pointer argument since we may update it. */ static reg_errcode_t # ifdef RE_ENABLE_I18N build_range_exp (const reg_syntax_t syntax, bitset_t sbcset, re_charset_t *mbcset, Idx *range_alloc, const bracket_elem_t *start_elem, const bracket_elem_t *end_elem) # else /* not RE_ENABLE_I18N */ build_range_exp (const reg_syntax_t syntax, bitset_t sbcset, const bracket_elem_t *start_elem, const bracket_elem_t *end_elem) # endif /* not RE_ENABLE_I18N */ { unsigned int start_ch, end_ch; /* Equivalence Classes and Character Classes can't be a range start/end. */ if (BE (start_elem->type == EQUIV_CLASS || start_elem->type == CHAR_CLASS || end_elem->type == EQUIV_CLASS || end_elem->type == CHAR_CLASS, 0)) return REG_ERANGE; /* We can handle no multi character collating elements without libc support. */ if (BE ((start_elem->type == COLL_SYM && strlen ((char *) start_elem->opr.name) > 1) || (end_elem->type == COLL_SYM && strlen ((char *) end_elem->opr.name) > 1), 0)) return REG_ECOLLATE; # ifdef RE_ENABLE_I18N { wchar_t wc; wint_t start_wc; wint_t end_wc; start_ch = ((start_elem->type == SB_CHAR) ? start_elem->opr.ch : ((start_elem->type == COLL_SYM) ? start_elem->opr.name[0] : 0)); end_ch = ((end_elem->type == SB_CHAR) ? end_elem->opr.ch : ((end_elem->type == COLL_SYM) ? end_elem->opr.name[0] : 0)); start_wc = ((start_elem->type == SB_CHAR || start_elem->type == COLL_SYM) ? parse_byte (start_ch, mbcset) : start_elem->opr.wch); end_wc = ((end_elem->type == SB_CHAR || end_elem->type == COLL_SYM) ? parse_byte (end_ch, mbcset) : end_elem->opr.wch); if (start_wc == WEOF || end_wc == WEOF) return REG_ECOLLATE; else if (BE ((syntax & RE_NO_EMPTY_RANGES) && start_wc > end_wc, 0)) return REG_ERANGE; /* Got valid collation sequence values, add them as a new entry. However, for !_LIBC we have no collation elements: if the character set is single byte, the single byte character set that we build below suffices. parse_bracket_exp passes no MBCSET if dfa->mb_cur_max == 1. */ if (mbcset) { /* Check the space of the arrays. */ if (BE (*range_alloc == mbcset->nranges, 0)) { /* There is not enough space, need realloc. */ wchar_t *new_array_start, *new_array_end; Idx new_nranges; /* +1 in case of mbcset->nranges is 0. */ new_nranges = 2 * mbcset->nranges + 1; /* Use realloc since mbcset->range_starts and mbcset->range_ends are NULL if *range_alloc == 0. */ new_array_start = re_realloc (mbcset->range_starts, wchar_t, new_nranges); new_array_end = re_realloc (mbcset->range_ends, wchar_t, new_nranges); if (BE (new_array_start == NULL || new_array_end == NULL, 0)) { re_free (new_array_start); re_free (new_array_end); return REG_ESPACE; } mbcset->range_starts = new_array_start; mbcset->range_ends = new_array_end; *range_alloc = new_nranges; } mbcset->range_starts[mbcset->nranges] = start_wc; mbcset->range_ends[mbcset->nranges++] = end_wc; } /* Build the table for single byte characters. */ for (wc = 0; wc < SBC_MAX; ++wc) { if (start_wc <= wc && wc <= end_wc) bitset_set (sbcset, wc); } } # else /* not RE_ENABLE_I18N */ { unsigned int ch; start_ch = ((start_elem->type == SB_CHAR ) ? start_elem->opr.ch : ((start_elem->type == COLL_SYM) ? start_elem->opr.name[0] : 0)); end_ch = ((end_elem->type == SB_CHAR ) ? end_elem->opr.ch : ((end_elem->type == COLL_SYM) ? end_elem->opr.name[0] : 0)); if (start_ch > end_ch) return REG_ERANGE; /* Build the table for single byte characters. */ for (ch = 0; ch < SBC_MAX; ++ch) if (start_ch <= ch && ch <= end_ch) bitset_set (sbcset, ch); } # endif /* not RE_ENABLE_I18N */ return REG_NOERROR; } #endif /* not _LIBC */ #ifndef _LIBC /* Helper function for parse_bracket_exp only used in case of NOT _LIBC.. Build the collating element which is represented by NAME. The result are written to MBCSET and SBCSET. COLL_SYM_ALLOC is the allocated size of mbcset->coll_sym, is a pointer argument since we may update it. */ static reg_errcode_t # ifdef RE_ENABLE_I18N build_collating_symbol (bitset_t sbcset, re_charset_t *mbcset, Idx *coll_sym_alloc, const unsigned char *name) # else /* not RE_ENABLE_I18N */ build_collating_symbol (bitset_t sbcset, const unsigned char *name) # endif /* not RE_ENABLE_I18N */ { size_t name_len = strlen ((const char *) name); if (BE (name_len != 1, 0)) return REG_ECOLLATE; else { bitset_set (sbcset, name[0]); return REG_NOERROR; } } #endif /* not _LIBC */ /* This function parse bracket expression like "[abc]", "[a-c]", "[[.a-a.]]" etc. */ static bin_tree_t * parse_bracket_exp (re_string_t *regexp, re_dfa_t *dfa, re_token_t *token, reg_syntax_t syntax, reg_errcode_t *err) { #ifdef _LIBC const unsigned char *collseqmb; const char *collseqwc; uint32_t nrules; int32_t table_size; const int32_t *symb_table; const unsigned char *extra; /* Local function for parse_bracket_exp used in _LIBC environment. Seek the collating symbol entry corresponding to NAME. Return the index of the symbol in the SYMB_TABLE, or -1 if not found. */ auto inline int32_t __attribute__ ((always_inline)) seek_collating_symbol_entry (const unsigned char *name, size_t name_len) { int32_t elem; for (elem = 0; elem < table_size; elem++) if (symb_table[2 * elem] != 0) { int32_t idx = symb_table[2 * elem + 1]; /* Skip the name of collating element name. */ idx += 1 + extra[idx]; if (/* Compare the length of the name. */ name_len == extra[idx] /* Compare the name. */ && memcmp (name, &extra[idx + 1], name_len) == 0) /* Yep, this is the entry. */ return elem; } return -1; } /* Local function for parse_bracket_exp used in _LIBC environment. Look up the collation sequence value of BR_ELEM. Return the value if succeeded, UINT_MAX otherwise. */ auto inline unsigned int __attribute__ ((always_inline)) lookup_collation_sequence_value (bracket_elem_t *br_elem) { if (br_elem->type == SB_CHAR) { /* if (MB_CUR_MAX == 1) */ if (nrules == 0) return collseqmb[br_elem->opr.ch]; else { wint_t wc = __btowc (br_elem->opr.ch); return __collseq_table_lookup (collseqwc, wc); } } else if (br_elem->type == MB_CHAR) { if (nrules != 0) return __collseq_table_lookup (collseqwc, br_elem->opr.wch); } else if (br_elem->type == COLL_SYM) { size_t sym_name_len = strlen ((char *) br_elem->opr.name); if (nrules != 0) { int32_t elem, idx; elem = seek_collating_symbol_entry (br_elem->opr.name, sym_name_len); if (elem != -1) { /* We found the entry. */ idx = symb_table[2 * elem + 1]; /* Skip the name of collating element name. */ idx += 1 + extra[idx]; /* Skip the byte sequence of the collating element. */ idx += 1 + extra[idx]; /* Adjust for the alignment. */ idx = (idx + 3) & ~3; /* Skip the multibyte collation sequence value. */ idx += sizeof (unsigned int); /* Skip the wide char sequence of the collating element. */ idx += sizeof (unsigned int) * (1 + *(unsigned int *) (extra + idx)); /* Return the collation sequence value. */ return *(unsigned int *) (extra + idx); } else if (sym_name_len == 1) { /* No valid character. Match it as a single byte character. */ return collseqmb[br_elem->opr.name[0]]; } } else if (sym_name_len == 1) return collseqmb[br_elem->opr.name[0]]; } return UINT_MAX; } /* Local function for parse_bracket_exp used in _LIBC environment. Build the range expression which starts from START_ELEM, and ends at END_ELEM. The result are written to MBCSET and SBCSET. RANGE_ALLOC is the allocated size of mbcset->range_starts, and mbcset->range_ends, is a pointer argument since we may update it. */ auto inline reg_errcode_t __attribute__ ((always_inline)) build_range_exp (bitset_t sbcset, re_charset_t *mbcset, int *range_alloc, bracket_elem_t *start_elem, bracket_elem_t *end_elem) { unsigned int ch; uint32_t start_collseq; uint32_t end_collseq; /* Equivalence Classes and Character Classes can't be a range start/end. */ if (BE (start_elem->type == EQUIV_CLASS || start_elem->type == CHAR_CLASS || end_elem->type == EQUIV_CLASS || end_elem->type == CHAR_CLASS, 0)) return REG_ERANGE; /* FIXME: Implement rational ranges here, too. */ start_collseq = lookup_collation_sequence_value (start_elem); end_collseq = lookup_collation_sequence_value (end_elem); /* Check start/end collation sequence values. */ if (BE (start_collseq == UINT_MAX || end_collseq == UINT_MAX, 0)) return REG_ECOLLATE; if (BE ((syntax & RE_NO_EMPTY_RANGES) && start_collseq > end_collseq, 0)) return REG_ERANGE; /* Got valid collation sequence values, add them as a new entry. However, if we have no collation elements, and the character set is single byte, the single byte character set that we build below suffices. */ if (nrules > 0 || dfa->mb_cur_max > 1) { /* Check the space of the arrays. */ if (BE (*range_alloc == mbcset->nranges, 0)) { /* There is not enough space, need realloc. */ uint32_t *new_array_start; uint32_t *new_array_end; Idx new_nranges; /* +1 in case of mbcset->nranges is 0. */ new_nranges = 2 * mbcset->nranges + 1; new_array_start = re_realloc (mbcset->range_starts, uint32_t, new_nranges); new_array_end = re_realloc (mbcset->range_ends, uint32_t, new_nranges); if (BE (new_array_start == NULL || new_array_end == NULL, 0)) return REG_ESPACE; mbcset->range_starts = new_array_start; mbcset->range_ends = new_array_end; *range_alloc = new_nranges; } mbcset->range_starts[mbcset->nranges] = start_collseq; mbcset->range_ends[mbcset->nranges++] = end_collseq; } /* Build the table for single byte characters. */ for (ch = 0; ch < SBC_MAX; ch++) { uint32_t ch_collseq; /* if (MB_CUR_MAX == 1) */ if (nrules == 0) ch_collseq = collseqmb[ch]; else ch_collseq = __collseq_table_lookup (collseqwc, __btowc (ch)); if (start_collseq <= ch_collseq && ch_collseq <= end_collseq) bitset_set (sbcset, ch); } return REG_NOERROR; } /* Local function for parse_bracket_exp used in _LIBC environment. Build the collating element which is represented by NAME. The result are written to MBCSET and SBCSET. COLL_SYM_ALLOC is the allocated size of mbcset->coll_sym, is a pointer argument since we may update it. */ auto inline reg_errcode_t __attribute__ ((always_inline)) build_collating_symbol (bitset_t sbcset, re_charset_t *mbcset, Idx *coll_sym_alloc, const unsigned char *name) { int32_t elem, idx; size_t name_len = strlen ((const char *) name); if (nrules != 0) { elem = seek_collating_symbol_entry (name, name_len); if (elem != -1) { /* We found the entry. */ idx = symb_table[2 * elem + 1]; /* Skip the name of collating element name. */ idx += 1 + extra[idx]; } else if (name_len == 1) { /* No valid character, treat it as a normal character. */ bitset_set (sbcset, name[0]); return REG_NOERROR; } else return REG_ECOLLATE; /* Got valid collation sequence, add it as a new entry. */ /* Check the space of the arrays. */ if (BE (*coll_sym_alloc == mbcset->ncoll_syms, 0)) { /* Not enough, realloc it. */ /* +1 in case of mbcset->ncoll_syms is 0. */ Idx new_coll_sym_alloc = 2 * mbcset->ncoll_syms + 1; /* Use realloc since mbcset->coll_syms is NULL if *alloc == 0. */ int32_t *new_coll_syms = re_realloc (mbcset->coll_syms, int32_t, new_coll_sym_alloc); if (BE (new_coll_syms == NULL, 0)) return REG_ESPACE; mbcset->coll_syms = new_coll_syms; *coll_sym_alloc = new_coll_sym_alloc; } mbcset->coll_syms[mbcset->ncoll_syms++] = idx; return REG_NOERROR; } else { if (BE (name_len != 1, 0)) return REG_ECOLLATE; else { bitset_set (sbcset, name[0]); return REG_NOERROR; } } } #endif re_token_t br_token; re_bitset_ptr_t sbcset; #ifdef RE_ENABLE_I18N re_charset_t *mbcset; Idx coll_sym_alloc = 0, range_alloc = 0, mbchar_alloc = 0; Idx equiv_class_alloc = 0, char_class_alloc = 0; #endif /* not RE_ENABLE_I18N */ bool non_match = false; bin_tree_t *work_tree; int token_len; bool first_round = true; #ifdef _LIBC collseqmb = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQMB); nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules) { /* if (MB_CUR_MAX > 1) */ collseqwc = _NL_CURRENT (LC_COLLATE, _NL_COLLATE_COLLSEQWC); table_size = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_SYMB_HASH_SIZEMB); symb_table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_TABLEMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_SYMB_EXTRAMB); } #endif sbcset = (re_bitset_ptr_t) calloc (sizeof (bitset_t), 1); #ifdef RE_ENABLE_I18N mbcset = (re_charset_t *) calloc (sizeof (re_charset_t), 1); #endif /* RE_ENABLE_I18N */ #ifdef RE_ENABLE_I18N if (BE (sbcset == NULL || mbcset == NULL, 0)) #else if (BE (sbcset == NULL, 0)) #endif /* RE_ENABLE_I18N */ { re_free (sbcset); #ifdef RE_ENABLE_I18N re_free (mbcset); #endif *err = REG_ESPACE; return NULL; } token_len = peek_token_bracket (token, regexp, syntax); if (BE (token->type == END_OF_RE, 0)) { *err = REG_BADPAT; goto parse_bracket_exp_free_return; } if (token->type == OP_NON_MATCH_LIST) { #ifdef RE_ENABLE_I18N mbcset->non_match = 1; #endif /* not RE_ENABLE_I18N */ non_match = true; if (syntax & RE_HAT_LISTS_NOT_NEWLINE) bitset_set (sbcset, '\n'); re_string_skip_bytes (regexp, token_len); /* Skip a token. */ token_len = peek_token_bracket (token, regexp, syntax); if (BE (token->type == END_OF_RE, 0)) { *err = REG_BADPAT; goto parse_bracket_exp_free_return; } } /* We treat the first ']' as a normal character. */ if (token->type == OP_CLOSE_BRACKET) token->type = CHARACTER; while (1) { bracket_elem_t start_elem, end_elem; unsigned char start_name_buf[BRACKET_NAME_BUF_SIZE]; unsigned char end_name_buf[BRACKET_NAME_BUF_SIZE]; reg_errcode_t ret; int token_len2 = 0; bool is_range_exp = false; re_token_t token2; start_elem.opr.name = start_name_buf; start_elem.type = COLL_SYM; ret = parse_bracket_element (&start_elem, regexp, token, token_len, dfa, syntax, first_round); if (BE (ret != REG_NOERROR, 0)) { *err = ret; goto parse_bracket_exp_free_return; } first_round = false; /* Get information about the next token. We need it in any case. */ token_len = peek_token_bracket (token, regexp, syntax); /* Do not check for ranges if we know they are not allowed. */ if (start_elem.type != CHAR_CLASS && start_elem.type != EQUIV_CLASS) { if (BE (token->type == END_OF_RE, 0)) { *err = REG_EBRACK; goto parse_bracket_exp_free_return; } if (token->type == OP_CHARSET_RANGE) { re_string_skip_bytes (regexp, token_len); /* Skip '-'. */ token_len2 = peek_token_bracket (&token2, regexp, syntax); if (BE (token2.type == END_OF_RE, 0)) { *err = REG_EBRACK; goto parse_bracket_exp_free_return; } if (token2.type == OP_CLOSE_BRACKET) { /* We treat the last '-' as a normal character. */ re_string_skip_bytes (regexp, -token_len); token->type = CHARACTER; } else is_range_exp = true; } } if (is_range_exp == true) { end_elem.opr.name = end_name_buf; end_elem.type = COLL_SYM; ret = parse_bracket_element (&end_elem, regexp, &token2, token_len2, dfa, syntax, true); if (BE (ret != REG_NOERROR, 0)) { *err = ret; goto parse_bracket_exp_free_return; } token_len = peek_token_bracket (token, regexp, syntax); #ifdef _LIBC *err = build_range_exp (sbcset, mbcset, &range_alloc, &start_elem, &end_elem); #else # ifdef RE_ENABLE_I18N *err = build_range_exp (syntax, sbcset, dfa->mb_cur_max > 1 ? mbcset : NULL, &range_alloc, &start_elem, &end_elem); # else *err = build_range_exp (syntax, sbcset, &start_elem, &end_elem); # endif #endif /* RE_ENABLE_I18N */ if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; } else { switch (start_elem.type) { case SB_CHAR: bitset_set (sbcset, start_elem.opr.ch); break; #ifdef RE_ENABLE_I18N case MB_CHAR: /* Check whether the array has enough space. */ if (BE (mbchar_alloc == mbcset->nmbchars, 0)) { wchar_t *new_mbchars; /* Not enough, realloc it. */ /* +1 in case of mbcset->nmbchars is 0. */ mbchar_alloc = 2 * mbcset->nmbchars + 1; /* Use realloc since array is NULL if *alloc == 0. */ new_mbchars = re_realloc (mbcset->mbchars, wchar_t, mbchar_alloc); if (BE (new_mbchars == NULL, 0)) goto parse_bracket_exp_espace; mbcset->mbchars = new_mbchars; } mbcset->mbchars[mbcset->nmbchars++] = start_elem.opr.wch; break; #endif /* RE_ENABLE_I18N */ case EQUIV_CLASS: *err = build_equiv_class (sbcset, #ifdef RE_ENABLE_I18N mbcset, &equiv_class_alloc, #endif /* RE_ENABLE_I18N */ start_elem.opr.name); if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; break; case COLL_SYM: *err = build_collating_symbol (sbcset, #ifdef RE_ENABLE_I18N mbcset, &coll_sym_alloc, #endif /* RE_ENABLE_I18N */ start_elem.opr.name); if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; break; case CHAR_CLASS: *err = build_charclass (regexp->trans, sbcset, #ifdef RE_ENABLE_I18N mbcset, &char_class_alloc, #endif /* RE_ENABLE_I18N */ (const char *) start_elem.opr.name, syntax); if (BE (*err != REG_NOERROR, 0)) goto parse_bracket_exp_free_return; break; default: assert (0); break; } } if (BE (token->type == END_OF_RE, 0)) { *err = REG_EBRACK; goto parse_bracket_exp_free_return; } if (token->type == OP_CLOSE_BRACKET) break; } re_string_skip_bytes (regexp, token_len); /* Skip a token. */ /* If it is non-matching list. */ if (non_match) bitset_not (sbcset); #ifdef RE_ENABLE_I18N /* Ensure only single byte characters are set. */ if (dfa->mb_cur_max > 1) bitset_mask (sbcset, dfa->sb_char); if (mbcset->nmbchars || mbcset->ncoll_syms || mbcset->nequiv_classes || mbcset->nranges || (dfa->mb_cur_max > 1 && (mbcset->nchar_classes || mbcset->non_match))) { bin_tree_t *mbc_tree; int sbc_idx; /* Build a tree for complex bracket. */ dfa->has_mb_node = 1; br_token.type = COMPLEX_BRACKET; br_token.opr.mbcset = mbcset; mbc_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (mbc_tree == NULL, 0)) goto parse_bracket_exp_espace; for (sbc_idx = 0; sbc_idx < BITSET_WORDS; ++sbc_idx) if (sbcset[sbc_idx]) break; /* If there are no bits set in sbcset, there is no point of having both SIMPLE_BRACKET and COMPLEX_BRACKET. */ if (sbc_idx < BITSET_WORDS) { /* Build a tree for simple bracket. */ br_token.type = SIMPLE_BRACKET; br_token.opr.sbcset = sbcset; work_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (work_tree == NULL, 0)) goto parse_bracket_exp_espace; /* Then join them by ALT node. */ work_tree = create_tree (dfa, work_tree, mbc_tree, OP_ALT); if (BE (work_tree == NULL, 0)) goto parse_bracket_exp_espace; } else { re_free (sbcset); work_tree = mbc_tree; } } else #endif /* not RE_ENABLE_I18N */ { #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* Build a tree for simple bracket. */ br_token.type = SIMPLE_BRACKET; br_token.opr.sbcset = sbcset; work_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (work_tree == NULL, 0)) goto parse_bracket_exp_espace; } return work_tree; parse_bracket_exp_espace: *err = REG_ESPACE; parse_bracket_exp_free_return: re_free (sbcset); #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* RE_ENABLE_I18N */ return NULL; } /* Parse an element in the bracket expression. */ static reg_errcode_t parse_bracket_element (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token, int token_len, re_dfa_t *dfa, reg_syntax_t syntax, bool accept_hyphen) { #ifdef RE_ENABLE_I18N int cur_char_size; cur_char_size = re_string_char_size_at (regexp, re_string_cur_idx (regexp)); if (cur_char_size > 1) { elem->type = MB_CHAR; elem->opr.wch = re_string_wchar_at (regexp, re_string_cur_idx (regexp)); re_string_skip_bytes (regexp, cur_char_size); return REG_NOERROR; } #endif /* RE_ENABLE_I18N */ re_string_skip_bytes (regexp, token_len); /* Skip a token. */ if (token->type == OP_OPEN_COLL_ELEM || token->type == OP_OPEN_CHAR_CLASS || token->type == OP_OPEN_EQUIV_CLASS) return parse_bracket_symbol (elem, regexp, token); if (BE (token->type == OP_CHARSET_RANGE, 0) && !accept_hyphen) { /* A '-' must only appear as anything but a range indicator before the closing bracket. Everything else is an error. */ re_token_t token2; (void) peek_token_bracket (&token2, regexp, syntax); if (token2.type != OP_CLOSE_BRACKET) /* The actual error value is not standardized since this whole case is undefined. But ERANGE makes good sense. */ return REG_ERANGE; } elem->type = SB_CHAR; elem->opr.ch = token->opr.c; return REG_NOERROR; } /* Parse a bracket symbol in the bracket expression. Bracket symbols are such as [::], [..], and [==]. */ static reg_errcode_t parse_bracket_symbol (bracket_elem_t *elem, re_string_t *regexp, re_token_t *token) { unsigned char ch, delim = token->opr.c; int i = 0; if (re_string_eoi(regexp)) return REG_EBRACK; for (;; ++i) { if (i >= BRACKET_NAME_BUF_SIZE) return REG_EBRACK; if (token->type == OP_OPEN_CHAR_CLASS) ch = re_string_fetch_byte_case (regexp); else ch = re_string_fetch_byte (regexp); if (re_string_eoi(regexp)) return REG_EBRACK; if (ch == delim && re_string_peek_byte (regexp, 0) == ']') break; elem->opr.name[i] = ch; } re_string_skip_bytes (regexp, 1); elem->opr.name[i] = '\0'; switch (token->type) { case OP_OPEN_COLL_ELEM: elem->type = COLL_SYM; break; case OP_OPEN_EQUIV_CLASS: elem->type = EQUIV_CLASS; break; case OP_OPEN_CHAR_CLASS: elem->type = CHAR_CLASS; break; default: break; } return REG_NOERROR; } /* Helper function for parse_bracket_exp. Build the equivalence class which is represented by NAME. The result are written to MBCSET and SBCSET. EQUIV_CLASS_ALLOC is the allocated size of mbcset->equiv_classes, is a pointer argument since we may update it. */ static reg_errcode_t #ifdef RE_ENABLE_I18N build_equiv_class (bitset_t sbcset, re_charset_t *mbcset, Idx *equiv_class_alloc, const unsigned char *name) #else /* not RE_ENABLE_I18N */ build_equiv_class (bitset_t sbcset, const unsigned char *name) #endif /* not RE_ENABLE_I18N */ { #ifdef _LIBC uint32_t nrules = _NL_CURRENT_WORD (LC_COLLATE, _NL_COLLATE_NRULES); if (nrules != 0) { const int32_t *table, *indirect; const unsigned char *weights, *extra, *cp; unsigned char char_buf[2]; int32_t idx1, idx2; unsigned int ch; size_t len; /* Calculate the index for equivalence class. */ cp = name; table = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_TABLEMB); weights = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_WEIGHTMB); extra = (const unsigned char *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_EXTRAMB); indirect = (const int32_t *) _NL_CURRENT (LC_COLLATE, _NL_COLLATE_INDIRECTMB); idx1 = findidx (table, indirect, extra, &cp, -1); if (BE (idx1 == 0 || *cp != '\0', 0)) /* This isn't a valid character. */ return REG_ECOLLATE; /* Build single byte matching table for this equivalence class. */ len = weights[idx1 & 0xffffff]; for (ch = 0; ch < SBC_MAX; ++ch) { char_buf[0] = ch; cp = char_buf; idx2 = findidx (table, indirect, extra, &cp, 1); /* idx2 = table[ch]; */ if (idx2 == 0) /* This isn't a valid character. */ continue; /* Compare only if the length matches and the collation rule index is the same. */ if (len == weights[idx2 & 0xffffff] && (idx1 >> 24) == (idx2 >> 24)) { int cnt = 0; while (cnt <= len && weights[(idx1 & 0xffffff) + 1 + cnt] == weights[(idx2 & 0xffffff) + 1 + cnt]) ++cnt; if (cnt > len) bitset_set (sbcset, ch); } } /* Check whether the array has enough space. */ if (BE (*equiv_class_alloc == mbcset->nequiv_classes, 0)) { /* Not enough, realloc it. */ /* +1 in case of mbcset->nequiv_classes is 0. */ Idx new_equiv_class_alloc = 2 * mbcset->nequiv_classes + 1; /* Use realloc since the array is NULL if *alloc == 0. */ int32_t *new_equiv_classes = re_realloc (mbcset->equiv_classes, int32_t, new_equiv_class_alloc); if (BE (new_equiv_classes == NULL, 0)) return REG_ESPACE; mbcset->equiv_classes = new_equiv_classes; *equiv_class_alloc = new_equiv_class_alloc; } mbcset->equiv_classes[mbcset->nequiv_classes++] = idx1; } else #endif /* _LIBC */ { if (BE (strlen ((const char *) name) != 1, 0)) return REG_ECOLLATE; bitset_set (sbcset, *name); } return REG_NOERROR; } /* Helper function for parse_bracket_exp. Build the character class which is represented by NAME. The result are written to MBCSET and SBCSET. CHAR_CLASS_ALLOC is the allocated size of mbcset->char_classes, is a pointer argument since we may update it. */ static reg_errcode_t #ifdef RE_ENABLE_I18N build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, re_charset_t *mbcset, Idx *char_class_alloc, const char *class_name, reg_syntax_t syntax) #else /* not RE_ENABLE_I18N */ build_charclass (RE_TRANSLATE_TYPE trans, bitset_t sbcset, const char *class_name, reg_syntax_t syntax) #endif /* not RE_ENABLE_I18N */ { int i; const char *name = class_name; /* In case of REG_ICASE "upper" and "lower" match the both of upper and lower cases. */ if ((syntax & RE_ICASE) && (strcmp (name, "upper") == 0 || strcmp (name, "lower") == 0)) name = "alpha"; #ifdef RE_ENABLE_I18N /* Check the space of the arrays. */ if (BE (*char_class_alloc == mbcset->nchar_classes, 0)) { /* Not enough, realloc it. */ /* +1 in case of mbcset->nchar_classes is 0. */ Idx new_char_class_alloc = 2 * mbcset->nchar_classes + 1; /* Use realloc since array is NULL if *alloc == 0. */ wctype_t *new_char_classes = re_realloc (mbcset->char_classes, wctype_t, new_char_class_alloc); if (BE (new_char_classes == NULL, 0)) return REG_ESPACE; mbcset->char_classes = new_char_classes; *char_class_alloc = new_char_class_alloc; } mbcset->char_classes[mbcset->nchar_classes++] = __wctype (name); #endif /* RE_ENABLE_I18N */ #define BUILD_CHARCLASS_LOOP(ctype_func) \ do { \ if (BE (trans != NULL, 0)) \ { \ for (i = 0; i < SBC_MAX; ++i) \ if (ctype_func (i)) \ bitset_set (sbcset, trans[i]); \ } \ else \ { \ for (i = 0; i < SBC_MAX; ++i) \ if (ctype_func (i)) \ bitset_set (sbcset, i); \ } \ } while (0) if (strcmp (name, "alnum") == 0) BUILD_CHARCLASS_LOOP (isalnum); else if (strcmp (name, "cntrl") == 0) BUILD_CHARCLASS_LOOP (iscntrl); else if (strcmp (name, "lower") == 0) BUILD_CHARCLASS_LOOP (islower); else if (strcmp (name, "space") == 0) BUILD_CHARCLASS_LOOP (isspace); else if (strcmp (name, "alpha") == 0) BUILD_CHARCLASS_LOOP (isalpha); else if (strcmp (name, "digit") == 0) BUILD_CHARCLASS_LOOP (isdigit); else if (strcmp (name, "print") == 0) BUILD_CHARCLASS_LOOP (isprint); else if (strcmp (name, "upper") == 0) BUILD_CHARCLASS_LOOP (isupper); else if (strcmp (name, "blank") == 0) BUILD_CHARCLASS_LOOP (isblank); else if (strcmp (name, "graph") == 0) BUILD_CHARCLASS_LOOP (isgraph); else if (strcmp (name, "punct") == 0) BUILD_CHARCLASS_LOOP (ispunct); else if (strcmp (name, "xdigit") == 0) BUILD_CHARCLASS_LOOP (isxdigit); else return REG_ECTYPE; return REG_NOERROR; } static bin_tree_t * build_charclass_op (re_dfa_t *dfa, RE_TRANSLATE_TYPE trans, const char *class_name, const char *extra, bool non_match, reg_errcode_t *err) { re_bitset_ptr_t sbcset; #ifdef RE_ENABLE_I18N re_charset_t *mbcset; Idx alloc = 0; #endif /* not RE_ENABLE_I18N */ reg_errcode_t ret; re_token_t br_token; bin_tree_t *tree; sbcset = (re_bitset_ptr_t) calloc (sizeof (bitset_t), 1); if (BE (sbcset == NULL, 0)) { *err = REG_ESPACE; return NULL; } #ifdef RE_ENABLE_I18N mbcset = (re_charset_t *) calloc (sizeof (re_charset_t), 1); if (BE (mbcset == NULL, 0)) { re_free (sbcset); *err = REG_ESPACE; return NULL; } mbcset->non_match = non_match; #endif /* RE_ENABLE_I18N */ /* We don't care the syntax in this case. */ ret = build_charclass (trans, sbcset, #ifdef RE_ENABLE_I18N mbcset, &alloc, #endif /* RE_ENABLE_I18N */ class_name, 0); if (BE (ret != REG_NOERROR, 0)) { re_free (sbcset); #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* RE_ENABLE_I18N */ *err = ret; return NULL; } /* \w match '_' also. */ for (; *extra; extra++) bitset_set (sbcset, *extra); /* If it is non-matching list. */ if (non_match) bitset_not (sbcset); #ifdef RE_ENABLE_I18N /* Ensure only single byte characters are set. */ if (dfa->mb_cur_max > 1) bitset_mask (sbcset, dfa->sb_char); #endif /* Build a tree for simple bracket. */ #if defined GCC_LINT || defined lint memset (&br_token, 0, sizeof br_token); #endif br_token.type = SIMPLE_BRACKET; br_token.opr.sbcset = sbcset; tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (tree == NULL, 0)) goto build_word_op_espace; #ifdef RE_ENABLE_I18N if (dfa->mb_cur_max > 1) { bin_tree_t *mbc_tree; /* Build a tree for complex bracket. */ br_token.type = COMPLEX_BRACKET; br_token.opr.mbcset = mbcset; dfa->has_mb_node = 1; mbc_tree = create_token_tree (dfa, NULL, NULL, &br_token); if (BE (mbc_tree == NULL, 0)) goto build_word_op_espace; /* Then join them by ALT node. */ tree = create_tree (dfa, tree, mbc_tree, OP_ALT); if (BE (mbc_tree != NULL, 1)) return tree; } else { free_charset (mbcset); return tree; } #else /* not RE_ENABLE_I18N */ return tree; #endif /* not RE_ENABLE_I18N */ build_word_op_espace: re_free (sbcset); #ifdef RE_ENABLE_I18N free_charset (mbcset); #endif /* RE_ENABLE_I18N */ *err = REG_ESPACE; return NULL; } /* This is intended for the expressions like "a{1,3}". Fetch a number from 'input', and return the number. Return -1 if the number field is empty like "{,1}". Return RE_DUP_MAX + 1 if the number field is too large. Return -2 if an error occurred. */ static Idx fetch_number (re_string_t *input, re_token_t *token, reg_syntax_t syntax) { Idx num = -1; unsigned char c; while (1) { fetch_token (token, input, syntax); c = token->opr.c; if (BE (token->type == END_OF_RE, 0)) return -2; if (token->type == OP_CLOSE_DUP_NUM || c == ',') break; num = ((token->type != CHARACTER || c < '0' || '9' < c || num == -2) ? -2 : num == -1 ? c - '0' : MIN (RE_DUP_MAX + 1, num * 10 + c - '0')); } return num; } #ifdef RE_ENABLE_I18N static void free_charset (re_charset_t *cset) { re_free (cset->mbchars); # ifdef _LIBC re_free (cset->coll_syms); re_free (cset->equiv_classes); re_free (cset->range_starts); re_free (cset->range_ends); # endif re_free (cset->char_classes); re_free (cset); } #endif /* RE_ENABLE_I18N */ /* Functions for binary tree operation. */ /* Create a tree node. */ static bin_tree_t * create_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, re_token_type_t type) { re_token_t t; #if defined GCC_LINT || defined lint memset (&t, 0, sizeof t); #endif t.type = type; return create_token_tree (dfa, left, right, &t); } static bin_tree_t * create_token_tree (re_dfa_t *dfa, bin_tree_t *left, bin_tree_t *right, const re_token_t *token) { bin_tree_t *tree; if (BE (dfa->str_tree_storage_idx == BIN_TREE_STORAGE_SIZE, 0)) { bin_tree_storage_t *storage = re_malloc (bin_tree_storage_t, 1); if (storage == NULL) return NULL; storage->next = dfa->str_tree_storage; dfa->str_tree_storage = storage; dfa->str_tree_storage_idx = 0; } tree = &dfa->str_tree_storage->data[dfa->str_tree_storage_idx++]; tree->parent = NULL; tree->left = left; tree->right = right; tree->token = *token; tree->token.duplicated = 0; tree->token.opt_subexp = 0; tree->first = NULL; tree->next = NULL; tree->node_idx = -1; if (left != NULL) left->parent = tree; if (right != NULL) right->parent = tree; return tree; } /* Mark the tree SRC as an optional subexpression. To be called from preorder or postorder. */ static reg_errcode_t mark_opt_subexp (void *extra, bin_tree_t *node) { Idx idx = (uintptr_t) extra; if (node->token.type == SUBEXP && node->token.opr.idx == idx) node->token.opt_subexp = 1; return REG_NOERROR; } /* Free the allocated memory inside NODE. */ static void free_token (re_token_t *node) { #ifdef RE_ENABLE_I18N if (node->type == COMPLEX_BRACKET && node->duplicated == 0) free_charset (node->opr.mbcset); else #endif /* RE_ENABLE_I18N */ if (node->type == SIMPLE_BRACKET && node->duplicated == 0) re_free (node->opr.sbcset); } /* Worker function for tree walking. Free the allocated memory inside NODE and its children. */ static reg_errcode_t free_tree (void *extra, bin_tree_t *node) { free_token (&node->token); return REG_NOERROR; } /* Duplicate the node SRC, and return new node. This is a preorder visit similar to the one implemented by the generic visitor, but we need more infrastructure to maintain two parallel trees --- so, it's easier to duplicate. */ static bin_tree_t * duplicate_tree (const bin_tree_t *root, re_dfa_t *dfa) { const bin_tree_t *node; bin_tree_t *dup_root; bin_tree_t **p_new = &dup_root, *dup_node = root->parent; for (node = root; ; ) { /* Create a new tree and link it back to the current parent. */ *p_new = create_token_tree (dfa, NULL, NULL, &node->token); if (*p_new == NULL) return NULL; (*p_new)->parent = dup_node; (*p_new)->token.duplicated = 1; dup_node = *p_new; /* Go to the left node, or up and to the right. */ if (node->left) { node = node->left; p_new = &dup_node->left; } else { const bin_tree_t *prev = NULL; while (node->right == prev || node->right == NULL) { prev = node; node = node->parent; dup_node = dup_node->parent; if (!node) return dup_root; } node = node->right; p_new = &dup_node->right; } } } gnuastro-0.5/bootstrapped/lib/rawmemchr.c0000644000175000017500000001220213217200021015527 00000000000000/* Searching in a string. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include /* Find the first occurrence of C in S. */ void * rawmemchr (const void *s, int c_in) { /* On 32-bit hardware, choosing longword to be a 32-bit unsigned long instead of a 64-bit uintmax_t tends to give better performance. On 64-bit hardware, unsigned long is generally 64 bits already. Change this typedef to experiment with performance. */ typedef unsigned long int longword; const unsigned char *char_ptr; const longword *longword_ptr; longword repeated_one; longword repeated_c; unsigned char c; c = (unsigned char) c_in; /* Handle the first few bytes by reading one byte at a time. Do this until CHAR_PTR is aligned on a longword boundary. */ for (char_ptr = (const unsigned char *) s; (size_t) char_ptr % sizeof (longword) != 0; ++char_ptr) if (*char_ptr == c) return (void *) char_ptr; longword_ptr = (const longword *) char_ptr; /* All these elucidatory comments refer to 4-byte longwords, but the theory applies equally well to any size longwords. */ /* Compute auxiliary longword values: repeated_one is a value which has a 1 in every byte. repeated_c has c in every byte. */ repeated_one = 0x01010101; repeated_c = c | (c << 8); repeated_c |= repeated_c << 16; if (0xffffffffU < (longword) -1) { repeated_one |= repeated_one << 31 << 1; repeated_c |= repeated_c << 31 << 1; if (8 < sizeof (longword)) { size_t i; for (i = 64; i < sizeof (longword) * 8; i *= 2) { repeated_one |= repeated_one << i; repeated_c |= repeated_c << i; } } } /* Instead of the traditional loop which tests each byte, we will test a longword at a time. The tricky part is testing if *any of the four* bytes in the longword in question are equal to NUL or c. We first use an xor with repeated_c. This reduces the task to testing whether *any of the four* bytes in longword1 is zero. We compute tmp = ((longword1 - repeated_one) & ~longword1) & (repeated_one << 7). That is, we perform the following operations: 1. Subtract repeated_one. 2. & ~longword1. 3. & a mask consisting of 0x80 in every byte. Consider what happens in each byte: - If a byte of longword1 is zero, step 1 and 2 transform it into 0xff, and step 3 transforms it into 0x80. A carry can also be propagated to more significant bytes. - If a byte of longword1 is nonzero, let its lowest 1 bit be at position k (0 <= k <= 7); so the lowest k bits are 0. After step 1, the byte ends in a single bit of value 0 and k bits of value 1. After step 2, the result is just k bits of value 1: 2^k - 1. After step 3, the result is 0. And no carry is produced. So, if longword1 has only non-zero bytes, tmp is zero. Whereas if longword1 has a zero byte, call j the position of the least significant zero byte. Then the result has a zero at positions 0, ..., j-1 and a 0x80 at position j. We cannot predict the result at the more significant bytes (positions j+1..3), but it does not matter since we already have a non-zero bit at position 8*j+7. The test whether any byte in longword1 is zero is equivalent to testing whether tmp is nonzero. This test can read beyond the end of a string, depending on where C_IN is encountered. However, this is considered safe since the initialization phase ensured that the read will be aligned, therefore, the read will not cross page boundaries and will not cause a fault. */ while (1) { longword longword1 = *longword_ptr ^ repeated_c; if ((((longword1 - repeated_one) & ~longword1) & (repeated_one << 7)) != 0) break; longword_ptr++; } char_ptr = (const unsigned char *) longword_ptr; /* At this point, we know that one of the sizeof (longword) bytes starting at char_ptr is == c. On little-endian machines, we could determine the first such byte without any further memory accesses, just by looking at the tmp result from the last loop iteration. But this does not work on big-endian machines. Choose code that works in both cases. */ char_ptr = (unsigned char *) longword_ptr; while (*char_ptr != c) char_ptr++; return (void *) char_ptr; } gnuastro-0.5/bootstrapped/lib/nl_langinfo.c0000644000175000017500000002202013217200021016027 00000000000000/* nl_langinfo() replacement: query locale dependent information. Copyright (C) 2007-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # include #endif /* Return the codeset of the current locale, if this is easily deducible. Otherwise, return "". */ static char * ctype_codeset (void) { static char buf[2 + 10 + 1]; char const *locale = setlocale (LC_CTYPE, NULL); char *codeset = buf; size_t codesetlen; codeset[0] = '\0'; if (locale && locale[0]) { /* If the locale name contains an encoding after the dot, return it. */ char *dot = strchr (locale, '.'); if (dot) { /* Look for the possible @... trailer and remove it, if any. */ char *codeset_start = dot + 1; char const *modifier = strchr (codeset_start, '@'); if (! modifier) codeset = codeset_start; else { codesetlen = modifier - codeset_start; if (codesetlen < sizeof buf) { codeset = memcpy (buf, codeset_start, codesetlen); codeset[codesetlen] = '\0'; } } } } #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* If setlocale is successful, it returns the number of the codepage, as a string. Otherwise, fall back on Windows API GetACP, which returns the locale's codepage as a number (although this doesn't change according to what the 'setlocale' call specified). Either way, prepend "CP" to make it a valid codeset name. */ codesetlen = strlen (codeset); if (0 < codesetlen && codesetlen < sizeof buf - 2) memmove (buf + 2, codeset, codesetlen + 1); else sprintf (buf + 2, "%u", GetACP ()); codeset = memcpy (buf, "CP", 2); #endif return codeset; } #if REPLACE_NL_LANGINFO /* Override nl_langinfo with support for added nl_item values. */ # undef nl_langinfo char * rpl_nl_langinfo (nl_item item) { switch (item) { # if GNULIB_defined_CODESET case CODESET: return ctype_codeset (); # endif # if GNULIB_defined_T_FMT_AMPM case T_FMT_AMPM: return (char *) "%I:%M:%S %p"; # endif # if GNULIB_defined_ERA case ERA: /* The format is not standardized. In glibc it is a sequence of strings of the form "direction:offset:start_date:end_date:era_name:era_format" with an empty string at the end. */ return (char *) ""; case ERA_D_FMT: /* The %Ex conversion in strftime behaves like %x if the locale does not have an alternative time format. */ item = D_FMT; break; case ERA_D_T_FMT: /* The %Ec conversion in strftime behaves like %c if the locale does not have an alternative time format. */ item = D_T_FMT; break; case ERA_T_FMT: /* The %EX conversion in strftime behaves like %X if the locale does not have an alternative time format. */ item = T_FMT; break; case ALT_DIGITS: /* The format is not standardized. In glibc it is a sequence of 10 strings, appended in memory. */ return (char *) "\0\0\0\0\0\0\0\0\0\0"; # endif # if GNULIB_defined_YESEXPR || !FUNC_NL_LANGINFO_YESEXPR_WORKS case YESEXPR: return (char *) "^[yY]"; case NOEXPR: return (char *) "^[nN]"; # endif default: break; } return nl_langinfo (item); } #else /* Provide nl_langinfo from scratch, either for native MS-Windows, or for old Unix platforms without locales, such as Linux libc5 or BeOS. */ # include char * nl_langinfo (nl_item item) { static char nlbuf[100]; struct tm tmm = { 0 }; switch (item) { /* nl_langinfo items of the LC_CTYPE category */ case CODESET: { char *codeset = ctype_codeset (); if (*codeset) return codeset; } # ifdef __BEOS__ return (char *) "UTF-8"; # else return (char *) "ISO-8859-1"; # endif /* nl_langinfo items of the LC_NUMERIC category */ case RADIXCHAR: return localeconv () ->decimal_point; case THOUSEP: return localeconv () ->thousands_sep; case GROUPING: return localeconv () ->grouping; /* nl_langinfo items of the LC_TIME category. TODO: Really use the locale. */ case D_T_FMT: case ERA_D_T_FMT: return (char *) "%a %b %e %H:%M:%S %Y"; case D_FMT: case ERA_D_FMT: return (char *) "%m/%d/%y"; case T_FMT: case ERA_T_FMT: return (char *) "%H:%M:%S"; case T_FMT_AMPM: return (char *) "%I:%M:%S %p"; case AM_STR: if (!strftime (nlbuf, sizeof nlbuf, "%p", &tmm)) return (char *) "AM"; return nlbuf; case PM_STR: tmm.tm_hour = 12; if (!strftime (nlbuf, sizeof nlbuf, "%p", &tmm)) return (char *) "PM"; return nlbuf; case DAY_1: case DAY_2: case DAY_3: case DAY_4: case DAY_5: case DAY_6: case DAY_7: { static char const days[][sizeof "Wednesday"] = { "Sunday", "Monday", "Tuesday", "Wednesday", "Thursday", "Friday", "Saturday" }; tmm.tm_wday = item - DAY_1; if (!strftime (nlbuf, sizeof nlbuf, "%A", &tmm)) return (char *) days[item - DAY_1]; return nlbuf; } case ABDAY_1: case ABDAY_2: case ABDAY_3: case ABDAY_4: case ABDAY_5: case ABDAY_6: case ABDAY_7: { static char const abdays[][sizeof "Sun"] = { "Sun", "Mon", "Tue", "Wed", "Thu", "Fri", "Sat" }; tmm.tm_wday = item - ABDAY_1; if (!strftime (nlbuf, sizeof nlbuf, "%a", &tmm)) return (char *) abdays[item - ABDAY_1]; return nlbuf; } case MON_1: case MON_2: case MON_3: case MON_4: case MON_5: case MON_6: case MON_7: case MON_8: case MON_9: case MON_10: case MON_11: case MON_12: { static char const months[][sizeof "September"] = { "January", "February", "March", "April", "May", "June", "July", "September", "October", "November", "December" }; tmm.tm_mon = item - MON_1; if (!strftime (nlbuf, sizeof nlbuf, "%B", &tmm)) return (char *) months[item - MON_1]; return nlbuf; } case ABMON_1: case ABMON_2: case ABMON_3: case ABMON_4: case ABMON_5: case ABMON_6: case ABMON_7: case ABMON_8: case ABMON_9: case ABMON_10: case ABMON_11: case ABMON_12: { static char const abmonths[][sizeof "Jan"] = { "Jan", "Feb", "Mar", "Apr", "May", "Jun", "Jul", "Sep", "Oct", "Nov", "Dec" }; tmm.tm_mon = item - ABMON_1; if (!strftime (nlbuf, sizeof nlbuf, "%b", &tmm)) return (char *) abmonths[item - ABMON_1]; return nlbuf; } case ERA: return (char *) ""; case ALT_DIGITS: return (char *) "\0\0\0\0\0\0\0\0\0\0"; /* nl_langinfo items of the LC_MONETARY category. */ case CRNCYSTR: return localeconv () ->currency_symbol; case INT_CURR_SYMBOL: return localeconv () ->int_curr_symbol; case MON_DECIMAL_POINT: return localeconv () ->mon_decimal_point; case MON_THOUSANDS_SEP: return localeconv () ->mon_thousands_sep; case MON_GROUPING: return localeconv () ->mon_grouping; case POSITIVE_SIGN: return localeconv () ->positive_sign; case NEGATIVE_SIGN: return localeconv () ->negative_sign; case FRAC_DIGITS: return & localeconv () ->frac_digits; case INT_FRAC_DIGITS: return & localeconv () ->int_frac_digits; case P_CS_PRECEDES: return & localeconv () ->p_cs_precedes; case N_CS_PRECEDES: return & localeconv () ->n_cs_precedes; case P_SEP_BY_SPACE: return & localeconv () ->p_sep_by_space; case N_SEP_BY_SPACE: return & localeconv () ->n_sep_by_space; case P_SIGN_POSN: return & localeconv () ->p_sign_posn; case N_SIGN_POSN: return & localeconv () ->n_sign_posn; /* nl_langinfo items of the LC_MESSAGES category TODO: Really use the locale. */ case YESEXPR: return (char *) "^[yY]"; case NOEXPR: return (char *) "^[nN]"; default: return (char *) ""; } } #endif gnuastro-0.5/bootstrapped/lib/msvc-nothrow.c0000644000175000017500000000251513217200021016216 00000000000000/* Wrappers that don't throw invalid parameter notifications with MSVC runtime libraries. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "msvc-nothrow.h" /* Get declarations of the native Windows API functions. */ #define WIN32_LEAN_AND_MEAN #include #if HAVE_MSVC_INVALID_PARAMETER_HANDLER # include "msvc-inval.h" #endif #undef _get_osfhandle #if HAVE_MSVC_INVALID_PARAMETER_HANDLER intptr_t _gl_nothrow_get_osfhandle (int fd) { intptr_t result; TRY_MSVC_INVAL { result = _get_osfhandle (fd); } CATCH_MSVC_INVAL { result = (intptr_t) INVALID_HANDLE_VALUE; } DONE_MSVC_INVAL; return result; } #endif gnuastro-0.5/bootstrapped/lib/msvc-inval.c0000644000175000017500000000751213217200021015631 00000000000000/* Invalid parameter handler for MSVC runtime libraries. Copyright (C) 2011-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include "msvc-inval.h" #if HAVE_MSVC_INVALID_PARAMETER_HANDLER \ && !(MSVC_INVALID_PARAMETER_HANDLING == SANE_LIBRARY_HANDLING) /* Get _invalid_parameter_handler type and _set_invalid_parameter_handler declaration. */ # include # if MSVC_INVALID_PARAMETER_HANDLING == DEFAULT_HANDLING static void __cdecl gl_msvc_invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { } # else /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include # if defined _MSC_VER static void __cdecl gl_msvc_invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { RaiseException (STATUS_GNULIB_INVALID_PARAMETER, 0, 0, NULL); } # else /* An index to thread-local storage. */ static DWORD tls_index; static int tls_initialized /* = 0 */; /* Used as a fallback only. */ static struct gl_msvc_inval_per_thread not_per_thread; struct gl_msvc_inval_per_thread * gl_msvc_inval_current (void) { if (!tls_initialized) { tls_index = TlsAlloc (); tls_initialized = 1; } if (tls_index == TLS_OUT_OF_INDEXES) /* TlsAlloc had failed. */ return ¬_per_thread; else { struct gl_msvc_inval_per_thread *pointer = (struct gl_msvc_inval_per_thread *) TlsGetValue (tls_index); if (pointer == NULL) { /* First call. Allocate a new 'struct gl_msvc_inval_per_thread'. */ pointer = (struct gl_msvc_inval_per_thread *) malloc (sizeof (struct gl_msvc_inval_per_thread)); if (pointer == NULL) /* Could not allocate memory. Use the global storage. */ pointer = ¬_per_thread; TlsSetValue (tls_index, pointer); } return pointer; } } static void __cdecl gl_msvc_invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { struct gl_msvc_inval_per_thread *current = gl_msvc_inval_current (); if (current->restart_valid) longjmp (current->restart, 1); else /* An invalid parameter notification from outside the gnulib code. Give the caller a chance to intervene. */ RaiseException (STATUS_GNULIB_INVALID_PARAMETER, 0, 0, NULL); } # endif # endif static int gl_msvc_inval_initialized /* = 0 */; void gl_msvc_inval_ensure_handler (void) { if (gl_msvc_inval_initialized == 0) { _set_invalid_parameter_handler (gl_msvc_invalid_parameter_handler); gl_msvc_inval_initialized = 1; } } #endif gnuastro-0.5/bootstrapped/lib/mempcpy.c0000644000175000017500000000200313217200021015212 00000000000000/* Copy memory area and return pointer after last written byte. Copyright (C) 2003, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include /* Copy N bytes of SRC to DEST, return pointer to bytes after the last written byte. */ void * mempcpy (void *dest, const void *src, size_t n) { return (char *) memcpy (dest, src, n) + n; } gnuastro-0.5/bootstrapped/lib/memchr.c0000644000175000017500000001334713217200021015030 00000000000000/* Copyright (C) 1991, 1993, 1996-1997, 1999-2000, 2003-2004, 2006, 2008-2017 Free Software Foundation, Inc. Based on strlen implementation by Torbjorn Granlund (tege@sics.se), with help from Dan Sahlin (dan@sics.se) and commentary by Jim Blandy (jimb@ai.mit.edu); adaptation to memchr suggested by Dick Karpinski (dick@cca.ucsf.edu), and implemented by Roland McGrath (roland@ai.mit.edu). NOTE: The canonical source of this file is maintained with the GNU C Library. Bugs can be reported to bug-glibc@prep.ai.mit.edu. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _LIBC # include #endif #include #include #if defined _LIBC # include #else # define reg_char char #endif #include #if HAVE_BP_SYM_H || defined _LIBC # include #else # define BP_SYM(sym) sym #endif #undef __memchr #ifdef _LIBC # undef memchr #endif #ifndef weak_alias # define __memchr memchr #endif /* Search no more than N bytes of S for C. */ void * __memchr (void const *s, int c_in, size_t n) { /* On 32-bit hardware, choosing longword to be a 32-bit unsigned long instead of a 64-bit uintmax_t tends to give better performance. On 64-bit hardware, unsigned long is generally 64 bits already. Change this typedef to experiment with performance. */ typedef unsigned long int longword; const unsigned char *char_ptr; const longword *longword_ptr; longword repeated_one; longword repeated_c; unsigned reg_char c; c = (unsigned char) c_in; /* Handle the first few bytes by reading one byte at a time. Do this until CHAR_PTR is aligned on a longword boundary. */ for (char_ptr = (const unsigned char *) s; n > 0 && (size_t) char_ptr % sizeof (longword) != 0; --n, ++char_ptr) if (*char_ptr == c) return (void *) char_ptr; longword_ptr = (const longword *) char_ptr; /* All these elucidatory comments refer to 4-byte longwords, but the theory applies equally well to any size longwords. */ /* Compute auxiliary longword values: repeated_one is a value which has a 1 in every byte. repeated_c has c in every byte. */ repeated_one = 0x01010101; repeated_c = c | (c << 8); repeated_c |= repeated_c << 16; if (0xffffffffU < (longword) -1) { repeated_one |= repeated_one << 31 << 1; repeated_c |= repeated_c << 31 << 1; if (8 < sizeof (longword)) { size_t i; for (i = 64; i < sizeof (longword) * 8; i *= 2) { repeated_one |= repeated_one << i; repeated_c |= repeated_c << i; } } } /* Instead of the traditional loop which tests each byte, we will test a longword at a time. The tricky part is testing if *any of the four* bytes in the longword in question are equal to c. We first use an xor with repeated_c. This reduces the task to testing whether *any of the four* bytes in longword1 is zero. We compute tmp = ((longword1 - repeated_one) & ~longword1) & (repeated_one << 7). That is, we perform the following operations: 1. Subtract repeated_one. 2. & ~longword1. 3. & a mask consisting of 0x80 in every byte. Consider what happens in each byte: - If a byte of longword1 is zero, step 1 and 2 transform it into 0xff, and step 3 transforms it into 0x80. A carry can also be propagated to more significant bytes. - If a byte of longword1 is nonzero, let its lowest 1 bit be at position k (0 <= k <= 7); so the lowest k bits are 0. After step 1, the byte ends in a single bit of value 0 and k bits of value 1. After step 2, the result is just k bits of value 1: 2^k - 1. After step 3, the result is 0. And no carry is produced. So, if longword1 has only non-zero bytes, tmp is zero. Whereas if longword1 has a zero byte, call j the position of the least significant zero byte. Then the result has a zero at positions 0, ..., j-1 and a 0x80 at position j. We cannot predict the result at the more significant bytes (positions j+1..3), but it does not matter since we already have a non-zero bit at position 8*j+7. So, the test whether any byte in longword1 is zero is equivalent to testing whether tmp is nonzero. */ while (n >= sizeof (longword)) { longword longword1 = *longword_ptr ^ repeated_c; if ((((longword1 - repeated_one) & ~longword1) & (repeated_one << 7)) != 0) break; longword_ptr++; n -= sizeof (longword); } char_ptr = (const unsigned char *) longword_ptr; /* At this point, we know that either n < sizeof (longword), or one of the sizeof (longword) bytes starting at char_ptr is == c. On little-endian machines, we could determine the first such byte without any further memory accesses, just by looking at the tmp result from the last loop iteration. But this does not work on big-endian machines. Choose code that works in both cases. */ for (; n > 0; --n, ++char_ptr) { if (*char_ptr == c) return (void *) char_ptr; } return NULL; } #ifdef weak_alias weak_alias (__memchr, BP_SYM (memchr)) #endif gnuastro-0.5/bootstrapped/lib/mbtowc.c0000644000175000017500000000164713217200021015050 00000000000000/* Convert multibyte character to wide character. Copyright (C) 2011-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include #include #include #include #include "mbtowc-impl.h" gnuastro-0.5/bootstrapped/lib/mbsinit.c0000644000175000017500000000453713217200021015223 00000000000000/* Test for initial conversion state. Copyright (C) 2008-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "verify.h" #if GNULIB_defined_mbstate_t /* Platforms that lack mbsinit() also lack mbrlen(), mbrtowc(), mbsrtowcs() and wcrtomb(), wcsrtombs(). We assume that - sizeof (mbstate_t) >= 4, - only stateless encodings are supported (such as UTF-8 and EUC-JP, but not ISO-2022 variants), - for each encoding, the number of bytes for a wide character is <= 4. (This maximum is attained for UTF-8, GB18030, EUC-TW.) We define the meaning of mbstate_t as follows: - In mb -> wc direction, mbstate_t's first byte contains the number of buffered bytes (in the range 0..3), followed by up to 3 buffered bytes. See mbrtowc.c. - In wc -> mb direction, mbstate_t contains no information. In other words, it is always in the initial state. */ verify (sizeof (mbstate_t) >= 4); int mbsinit (const mbstate_t *ps) { const char *pstate = (const char *)ps; return pstate == NULL || pstate[0] == 0; } #else int mbsinit (const mbstate_t *ps) { # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* Native Windows. */ # ifdef __MINGW32__ /* On mingw, 'mbstate_t' is defined as 'int'. */ return ps == NULL || *ps == 0; # else /* MSVC defines 'mbstate_t' as an 8-byte struct; the first 4-bytes matter. */ return ps == NULL || *(const unsigned int *)ps == 0; # endif # else /* Minix, HP-UX 11.00, Solaris 2.6, Interix, ... */ /* Maybe this definition works, maybe not... */ return ps == NULL || *(const char *)ps == 0; # endif } #endif gnuastro-0.5/bootstrapped/lib/mbrtowc.c0000644000175000017500000002545613217200021015236 00000000000000/* Convert multibyte character to wide character. Copyright (C) 1999-2002, 2005-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if C_LOCALE_MAYBE_EILSEQ # include "hard-locale.h" # include #endif #if GNULIB_defined_mbstate_t /* Implement mbrtowc() on top of mbtowc(). */ # include # include # include "localcharset.h" # include "streq.h" # include "verify.h" #ifndef FALLTHROUGH # if __GNUC__ < 7 # define FALLTHROUGH ((void) 0) # else # define FALLTHROUGH __attribute__ ((__fallthrough__)) # endif #endif verify (sizeof (mbstate_t) >= 4); static char internal_state[4]; size_t mbrtowc (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps) { char *pstate = (char *)ps; if (s == NULL) { pwc = NULL; s = ""; n = 1; } if (n == 0) return (size_t)(-2); /* Here n > 0. */ if (pstate == NULL) pstate = internal_state; { size_t nstate = pstate[0]; char buf[4]; const char *p; size_t m; switch (nstate) { case 0: p = s; m = n; break; case 3: buf[2] = pstate[3]; FALLTHROUGH; case 2: buf[1] = pstate[2]; FALLTHROUGH; case 1: buf[0] = pstate[1]; p = buf; m = nstate; buf[m++] = s[0]; if (n >= 2 && m < 4) { buf[m++] = s[1]; if (n >= 3 && m < 4) buf[m++] = s[2]; } break; default: errno = EINVAL; return (size_t)(-1); } /* Here m > 0. */ # if __GLIBC__ || defined __UCLIBC__ /* Work around bug */ mbtowc (NULL, NULL, 0); # endif { int res = mbtowc (pwc, p, m); if (res >= 0) { if (pwc != NULL && ((*pwc == 0) != (res == 0))) abort (); if (nstate >= (res > 0 ? res : 1)) abort (); res -= nstate; pstate[0] = 0; return res; } /* mbtowc does not distinguish between invalid and incomplete multibyte sequences. But mbrtowc needs to make this distinction. There are two possible approaches: - Use iconv() and its return value. - Use built-in knowledge about the possible encodings. Given the low quality of implementation of iconv() on the systems that lack mbrtowc(), we use the second approach. The possible encodings are: - 8-bit encodings, - EUC-JP, EUC-KR, GB2312, EUC-TW, BIG5, GB18030, SJIS, - UTF-8. Use specialized code for each. */ if (m >= 4 || m >= MB_CUR_MAX) goto invalid; /* Here MB_CUR_MAX > 1 and 0 < m < 4. */ { const char *encoding = locale_charset (); if (STREQ_OPT (encoding, "UTF-8", 'U', 'T', 'F', '-', '8', 0, 0, 0, 0)) { /* Cf. unistr/u8-mblen.c. */ unsigned char c = (unsigned char) p[0]; if (c >= 0xc2) { if (c < 0xe0) { if (m == 1) goto incomplete; } else if (c < 0xf0) { if (m == 1) goto incomplete; if (m == 2) { unsigned char c2 = (unsigned char) p[1]; if ((c2 ^ 0x80) < 0x40 && (c >= 0xe1 || c2 >= 0xa0) && (c != 0xed || c2 < 0xa0)) goto incomplete; } } else if (c <= 0xf4) { if (m == 1) goto incomplete; else /* m == 2 || m == 3 */ { unsigned char c2 = (unsigned char) p[1]; if ((c2 ^ 0x80) < 0x40 && (c >= 0xf1 || c2 >= 0x90) && (c < 0xf4 || (c == 0xf4 && c2 < 0x90))) { if (m == 2) goto incomplete; else /* m == 3 */ { unsigned char c3 = (unsigned char) p[2]; if ((c3 ^ 0x80) < 0x40) goto incomplete; } } } } } goto invalid; } /* As a reference for this code, you can use the GNU libiconv implementation. Look for uses of the RET_TOOFEW macro. */ if (STREQ_OPT (encoding, "EUC-JP", 'E', 'U', 'C', '-', 'J', 'P', 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0xa1 && c < 0xff) || c == 0x8e || c == 0x8f) goto incomplete; } if (m == 2) { unsigned char c = (unsigned char) p[0]; if (c == 0x8f) { unsigned char c2 = (unsigned char) p[1]; if (c2 >= 0xa1 && c2 < 0xff) goto incomplete; } } goto invalid; } if (STREQ_OPT (encoding, "EUC-KR", 'E', 'U', 'C', '-', 'K', 'R', 0, 0, 0) || STREQ_OPT (encoding, "GB2312", 'G', 'B', '2', '3', '1', '2', 0, 0, 0) || STREQ_OPT (encoding, "BIG5", 'B', 'I', 'G', '5', 0, 0, 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if (c >= 0xa1 && c < 0xff) goto incomplete; } goto invalid; } if (STREQ_OPT (encoding, "EUC-TW", 'E', 'U', 'C', '-', 'T', 'W', 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0xa1 && c < 0xff) || c == 0x8e) goto incomplete; } else /* m == 2 || m == 3 */ { unsigned char c = (unsigned char) p[0]; if (c == 0x8e) goto incomplete; } goto invalid; } if (STREQ_OPT (encoding, "GB18030", 'G', 'B', '1', '8', '0', '3', '0', 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0x90 && c <= 0xe3) || (c >= 0xf8 && c <= 0xfe)) goto incomplete; } else /* m == 2 || m == 3 */ { unsigned char c = (unsigned char) p[0]; if (c >= 0x90 && c <= 0xe3) { unsigned char c2 = (unsigned char) p[1]; if (c2 >= 0x30 && c2 <= 0x39) { if (m == 2) goto incomplete; else /* m == 3 */ { unsigned char c3 = (unsigned char) p[2]; if (c3 >= 0x81 && c3 <= 0xfe) goto incomplete; } } } } goto invalid; } if (STREQ_OPT (encoding, "SJIS", 'S', 'J', 'I', 'S', 0, 0, 0, 0, 0)) { if (m == 1) { unsigned char c = (unsigned char) p[0]; if ((c >= 0x81 && c <= 0x9f) || (c >= 0xe0 && c <= 0xea) || (c >= 0xf0 && c <= 0xf9)) goto incomplete; } goto invalid; } /* An unknown multibyte encoding. */ goto incomplete; } incomplete: { size_t k = nstate; /* Here 0 <= k < m < 4. */ pstate[++k] = s[0]; if (k < m) { pstate[++k] = s[1]; if (k < m) pstate[++k] = s[2]; } if (k != m) abort (); } pstate[0] = m; return (size_t)(-2); invalid: errno = EILSEQ; /* The conversion state is undefined, says POSIX. */ return (size_t)(-1); } } } #else /* Override the system's mbrtowc() function. */ # undef mbrtowc size_t rpl_mbrtowc (wchar_t *pwc, const char *s, size_t n, mbstate_t *ps) { size_t ret; wchar_t wc; # if MBRTOWC_NULL_ARG2_BUG || MBRTOWC_RETVAL_BUG || MBRTOWC_EMPTY_INPUT_BUG if (s == NULL) { pwc = NULL; s = ""; n = 1; } # endif # if MBRTOWC_EMPTY_INPUT_BUG if (n == 0) return (size_t) -2; # endif if (! pwc) pwc = &wc; # if MBRTOWC_RETVAL_BUG { static mbstate_t internal_state; /* Override mbrtowc's internal state. We cannot call mbsinit() on the hidden internal state, but we can call it on our variable. */ if (ps == NULL) ps = &internal_state; if (!mbsinit (ps)) { /* Parse the rest of the multibyte character byte for byte. */ size_t count = 0; for (; n > 0; s++, n--) { ret = mbrtowc (&wc, s, 1, ps); if (ret == (size_t)(-1)) return (size_t)(-1); count++; if (ret != (size_t)(-2)) { /* The multibyte character has been completed. */ *pwc = wc; return (wc == 0 ? 0 : count); } } return (size_t)(-2); } } # endif ret = mbrtowc (pwc, s, n, ps); # if MBRTOWC_NUL_RETVAL_BUG if (ret < (size_t) -2 && !*pwc) return 0; # endif # if C_LOCALE_MAYBE_EILSEQ if ((size_t) -2 <= ret && n != 0 && ! hard_locale (LC_CTYPE)) { unsigned char uc = *s; *pwc = uc; return 1; } # endif return ret; } #endif gnuastro-0.5/bootstrapped/lib/malloc.c0000644000175000017500000000273313217200021015021 00000000000000/* malloc() function that is glibc compatible. Copyright (C) 1997-1998, 2006-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* written by Jim Meyering and Bruno Haible */ #define _GL_USE_STDLIB_ALLOC 1 #include /* Only the AC_FUNC_MALLOC macro defines 'malloc' already in config.h. */ #ifdef malloc # define NEED_MALLOC_GNU 1 # undef malloc /* Whereas the gnulib module 'malloc-gnu' defines HAVE_MALLOC_GNU. */ #elif GNULIB_MALLOC_GNU && !HAVE_MALLOC_GNU # define NEED_MALLOC_GNU 1 #endif #include #include /* Allocate an N-byte block of memory from the heap. If N is zero, allocate a 1-byte block. */ void * rpl_malloc (size_t n) { void *result; #if NEED_MALLOC_GNU if (n == 0) n = 1; #endif result = malloc (n); #if !HAVE_MALLOC_POSIX if (result == NULL) errno = ENOMEM; #endif return result; } gnuastro-0.5/bootstrapped/lib/localeconv.c0000644000175000017500000000656313217200021015704 00000000000000/* Query locale dependent information for formatting numbers. Copyright (C) 2012-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if HAVE_STRUCT_LCONV_DECIMAL_POINT /* Override for platforms where 'struct lconv' lacks the int_p_*, int_n_* members. */ struct lconv * localeconv (void) { static struct lconv result; # undef lconv # undef localeconv struct lconv *sys_result = localeconv (); result.decimal_point = sys_result->decimal_point; result.thousands_sep = sys_result->thousands_sep; result.grouping = sys_result->grouping; result.mon_decimal_point = sys_result->mon_decimal_point; result.mon_thousands_sep = sys_result->mon_thousands_sep; result.mon_grouping = sys_result->mon_grouping; result.positive_sign = sys_result->positive_sign; result.negative_sign = sys_result->negative_sign; result.currency_symbol = sys_result->currency_symbol; result.frac_digits = sys_result->frac_digits; result.p_cs_precedes = sys_result->p_cs_precedes; result.p_sign_posn = sys_result->p_sign_posn; result.p_sep_by_space = sys_result->p_sep_by_space; result.n_cs_precedes = sys_result->n_cs_precedes; result.n_sign_posn = sys_result->n_sign_posn; result.n_sep_by_space = sys_result->n_sep_by_space; result.int_curr_symbol = sys_result->int_curr_symbol; result.int_frac_digits = sys_result->int_frac_digits; result.int_p_cs_precedes = sys_result->p_cs_precedes; result.int_p_sign_posn = sys_result->p_sign_posn; result.int_p_sep_by_space = sys_result->p_sep_by_space; result.int_n_cs_precedes = sys_result->n_cs_precedes; result.int_n_sign_posn = sys_result->n_sign_posn; result.int_n_sep_by_space = sys_result->n_sep_by_space; return &result; } #else /* Override for platforms where 'struct lconv' is a dummy. */ # include struct lconv * localeconv (void) { static /*const*/ struct lconv result = { /* decimal_point */ ".", /* thousands_sep */ "", /* grouping */ "", /* mon_decimal_point */ "", /* mon_thousands_sep */ "", /* mon_grouping */ "", /* positive_sign */ "", /* negative_sign */ "", /* currency_symbol */ "", /* frac_digits */ CHAR_MAX, /* p_cs_precedes */ CHAR_MAX, /* p_sign_posn */ CHAR_MAX, /* p_sep_by_space */ CHAR_MAX, /* n_cs_precedes */ CHAR_MAX, /* n_sign_posn */ CHAR_MAX, /* n_sep_by_space */ CHAR_MAX, /* int_curr_symbol */ "", /* int_frac_digits */ CHAR_MAX, /* int_p_cs_precedes */ CHAR_MAX, /* int_p_sign_posn */ CHAR_MAX, /* int_p_sep_by_space */ CHAR_MAX, /* int_n_cs_precedes */ CHAR_MAX, /* int_n_sign_posn */ CHAR_MAX, /* int_n_sep_by_space */ CHAR_MAX }; return &result; } #endif gnuastro-0.5/bootstrapped/lib/iswblank.c0000644000175000017500000000153213217200021015360 00000000000000/* Test wide character for being blank. Copyright (C) 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #include /* Specification. */ #include int iswblank (wint_t wc) { return wc == ' ' || wc == '\t'; } gnuastro-0.5/bootstrapped/lib/getopt1.c0000644000175000017500000000733113217200021015134 00000000000000/* getopt_long and getopt_long_only entry points for GNU getopt. Copyright (C) 1987-2017 Free Software Foundation, Inc. This file is part of the GNU C Library and is also part of gnulib. Patches to this file should be submitted to both projects. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _LIBC # include #endif #include "getopt.h" #include "getopt_int.h" int getopt_long (int argc, char *__getopt_argv_const *argv, const char *options, const struct option *long_options, int *opt_index) { return _getopt_internal (argc, (char **) argv, options, long_options, opt_index, 0, 0); } int _getopt_long_r (int argc, char **argv, const char *options, const struct option *long_options, int *opt_index, struct _getopt_data *d) { return _getopt_internal_r (argc, argv, options, long_options, opt_index, 0, d, 0); } /* Like getopt_long, but '-' as well as '--' can indicate a long option. If an option that starts with '-' (not '--') doesn't match a long option, but does match a short option, it is parsed as a short option instead. */ int getopt_long_only (int argc, char *__getopt_argv_const *argv, const char *options, const struct option *long_options, int *opt_index) { return _getopt_internal (argc, (char **) argv, options, long_options, opt_index, 1, 0); } int _getopt_long_only_r (int argc, char **argv, const char *options, const struct option *long_options, int *opt_index, struct _getopt_data *d) { return _getopt_internal_r (argc, argv, options, long_options, opt_index, 1, d, 0); } #ifdef TEST #include #include int main (int argc, char **argv) { int c; int digit_optind = 0; while (1) { int this_option_optind = optind ? optind : 1; int option_index = 0; static const struct option long_options[] = { {"add", 1, 0, 0}, {"append", 0, 0, 0}, {"delete", 1, 0, 0}, {"verbose", 0, 0, 0}, {"create", 0, 0, 0}, {"file", 1, 0, 0}, {0, 0, 0, 0} }; c = getopt_long (argc, argv, "abc:d:0123456789", long_options, &option_index); if (c == -1) break; switch (c) { case 0: printf ("option %s", long_options[option_index].name); if (optarg) printf (" with arg %s", optarg); printf ("\n"); break; case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': if (digit_optind != 0 && digit_optind != this_option_optind) printf ("digits occur in two different argv-elements.\n"); digit_optind = this_option_optind; printf ("option %c\n", c); break; case 'a': printf ("option a\n"); break; case 'b': printf ("option b\n"); break; case 'c': printf ("option c with value '%s'\n", optarg); break; case 'd': printf ("option d with value '%s'\n", optarg); break; case '?': break; default: printf ("?? getopt returned character code 0%o ??\n", c); } } if (optind < argc) { printf ("non-option ARGV-elements: "); while (optind < argc) printf ("%s ", argv[optind++]); printf ("\n"); } exit (0); } #endif /* TEST */ gnuastro-0.5/bootstrapped/lib/getopt.c0000644000175000017500000005711113217200021015054 00000000000000/* Getopt for GNU. Copyright (C) 1987-2017 Free Software Foundation, Inc. This file is part of the GNU C Library and is also part of gnulib. Patches to this file should be submitted to both projects. The GNU C Library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. The GNU C Library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with the GNU C Library; if not, see . */ #ifndef _LIBC # include #endif #include "getopt.h" #include #include #include #include #ifdef _LIBC /* When used as part of glibc, error printing must be done differently for standards compliance. getopt is not a cancellation point, so it must not call functions that are, and it is specified by an older standard than stdio locking, so it must not refer to functions in the "user namespace" related to stdio locking. Finally, it must use glibc's internal message translation so that the messages are looked up in the proper text domain. */ # include # define fprintf __fxprintf_nocancel # define flockfile(fp) _IO_flockfile (fp) # define funlockfile(fp) _IO_funlockfile (fp) #else # include "gettext.h" # define _(msgid) gettext (msgid) /* When used standalone, flockfile and funlockfile might not be available. */ # if (!defined _POSIX_THREAD_SAFE_FUNCTIONS \ || ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__)) # define flockfile(fp) /* nop */ # define funlockfile(fp) /* nop */ # endif /* When used standalone, do not attempt to use alloca. */ # define __libc_use_alloca(size) 0 # undef alloca # define alloca(size) (abort (), (void *)0) #endif /* This implementation of 'getopt' has three modes for handling options interspersed with non-option arguments. It can stop scanning for options at the first non-option argument encountered, as POSIX specifies. It can continue scanning for options after the first non-option argument, but permute 'argv' as it goes so that, after 'getopt' is done, all the options precede all the non-option arguments and 'optind' points to the first non-option argument. Or, it can report non-option arguments as if they were arguments to the option character '\x01'. The default behavior of 'getopt_long' is to permute the argument list. When this implementation is used standalone, the default behavior of 'getopt' is to stop at the first non-option argument, but when it is used as part of GNU libc it also permutes the argument list. In both cases, setting the environment variable POSIXLY_CORRECT to any value disables permutation. If the first character of the OPTSTRING argument to 'getopt' or 'getopt_long' is '+', both functions will stop at the first non-option argument. If it is '-', both functions will report non-option arguments as arguments to the option character '\x01'. */ #include "getopt_int.h" /* For communication from 'getopt' to the caller. When 'getopt' finds an option that takes an argument, the argument value is returned here. Also, when 'ordering' is RETURN_IN_ORDER, each non-option ARGV-element is returned here. */ char *optarg; /* Index in ARGV of the next element to be scanned. This is used for communication to and from the caller and for communication between successive calls to 'getopt'. On entry to 'getopt', zero means this is the first call; initialize. When 'getopt' returns -1, this is the index of the first of the non-option elements that the caller should itself scan. Otherwise, 'optind' communicates from one call to the next how much of ARGV has been scanned so far. */ /* 1003.2 says this must be 1 before any call. */ int optind = 1; /* Callers store zero here to inhibit the error message for unrecognized options. */ int opterr = 1; /* Set to an option character which was unrecognized. This must be initialized on some systems to avoid linking in the system's own getopt implementation. */ int optopt = '?'; /* Keep a global copy of all internal members of getopt_data. */ static struct _getopt_data getopt_data; /* Exchange two adjacent subsequences of ARGV. One subsequence is elements [first_nonopt,last_nonopt) which contains all the non-options that have been skipped so far. The other is elements [last_nonopt,optind), which contains all the options processed since those non-options were skipped. 'first_nonopt' and 'last_nonopt' are relocated so that they describe the new indices of the non-options in ARGV after they are moved. */ static void exchange (char **argv, struct _getopt_data *d) { int bottom = d->__first_nonopt; int middle = d->__last_nonopt; int top = d->optind; char *tem; /* Exchange the shorter segment with the far end of the longer segment. That puts the shorter segment into the right place. It leaves the longer segment in the right place overall, but it consists of two parts that need to be swapped next. */ while (top > middle && middle > bottom) { if (top - middle > middle - bottom) { /* Bottom segment is the short one. */ int len = middle - bottom; int i; /* Swap it with the top part of the top segment. */ for (i = 0; i < len; i++) { tem = argv[bottom + i]; argv[bottom + i] = argv[top - (middle - bottom) + i]; argv[top - (middle - bottom) + i] = tem; } /* Exclude the moved bottom segment from further swapping. */ top -= len; } else { /* Top segment is the short one. */ int len = top - middle; int i; /* Swap it with the bottom part of the bottom segment. */ for (i = 0; i < len; i++) { tem = argv[bottom + i]; argv[bottom + i] = argv[middle + i]; argv[middle + i] = tem; } /* Exclude the moved top segment from further swapping. */ bottom += len; } } /* Update records for the slots the non-options now occupy. */ d->__first_nonopt += (d->optind - d->__last_nonopt); d->__last_nonopt = d->optind; } /* Process the argument starting with d->__nextchar as a long option. d->optind should *not* have been advanced over this argument. If the value returned is -1, it was not actually a long option, the state is unchanged, and the argument should be processed as a set of short options (this can only happen when long_only is true). Otherwise, the option (and its argument, if any) have been consumed and the return value is the value to return from _getopt_internal_r. */ static int process_long_option (int argc, char **argv, const char *optstring, const struct option *longopts, int *longind, int long_only, struct _getopt_data *d, int print_errors, const char *prefix) { char *nameend; size_t namelen; const struct option *p; const struct option *pfound = NULL; int n_options; int option_index; for (nameend = d->__nextchar; *nameend && *nameend != '='; nameend++) /* Do nothing. */ ; namelen = nameend - d->__nextchar; /* First look for an exact match, counting the options as a side effect. */ for (p = longopts, n_options = 0; p->name; p++, n_options++) if (!strncmp (p->name, d->__nextchar, namelen) && namelen == strlen (p->name)) { /* Exact match found. */ pfound = p; option_index = n_options; break; } if (pfound == NULL) { /* Didn't find an exact match, so look for abbreviations. */ unsigned char *ambig_set = NULL; int ambig_malloced = 0; int ambig_fallback = 0; int indfound = -1; for (p = longopts, option_index = 0; p->name; p++, option_index++) if (!strncmp (p->name, d->__nextchar, namelen)) { if (pfound == NULL) { /* First nonexact match found. */ pfound = p; indfound = option_index; } else if (long_only || pfound->has_arg != p->has_arg || pfound->flag != p->flag || pfound->val != p->val) { /* Second or later nonexact match found. */ if (!ambig_fallback) { if (!print_errors) /* Don't waste effort tracking the ambig set if we're not going to print it anyway. */ ambig_fallback = 1; else if (!ambig_set) { if (__libc_use_alloca (n_options)) ambig_set = alloca (n_options); else if ((ambig_set = malloc (n_options)) == NULL) /* Fall back to simpler error message. */ ambig_fallback = 1; else ambig_malloced = 1; if (ambig_set) { memset (ambig_set, 0, n_options); ambig_set[indfound] = 1; } } if (ambig_set) ambig_set[option_index] = 1; } } } if (ambig_set || ambig_fallback) { if (print_errors) { if (ambig_fallback) fprintf (stderr, _("%s: option '%s%s' is ambiguous\n"), argv[0], prefix, d->__nextchar); else { flockfile (stderr); fprintf (stderr, _("%s: option '%s%s' is ambiguous; possibilities:"), argv[0], prefix, d->__nextchar); for (option_index = 0; option_index < n_options; option_index++) if (ambig_set[option_index]) fprintf (stderr, " '%s%s'", prefix, longopts[option_index].name); /* This must use 'fprintf' even though it's only printing a single character, so that it goes through __fxprintf_nocancel when compiled as part of glibc. */ fprintf (stderr, "\n"); funlockfile (stderr); } } if (ambig_malloced) free (ambig_set); d->__nextchar += strlen (d->__nextchar); d->optind++; d->optopt = 0; return '?'; } option_index = indfound; } if (pfound == NULL) { /* Can't find it as a long option. If this is not getopt_long_only, or the option starts with '--' or is not a valid short option, then it's an error. */ if (!long_only || argv[d->optind][1] == '-' || strchr (optstring, *d->__nextchar) == NULL) { if (print_errors) fprintf (stderr, _("%s: unrecognized option '%s%s'\n"), argv[0], prefix, d->__nextchar); d->__nextchar = NULL; d->optind++; d->optopt = 0; return '?'; } /* Otherwise interpret it as a short option. */ return -1; } /* We have found a matching long option. Consume it. */ d->optind++; d->__nextchar = NULL; if (*nameend) { /* Don't test has_arg with >, because some C compilers don't allow it to be used on enums. */ if (pfound->has_arg) d->optarg = nameend + 1; else { if (print_errors) fprintf (stderr, _("%s: option '%s%s' doesn't allow an argument\n"), argv[0], prefix, pfound->name); d->optopt = pfound->val; return '?'; } } else if (pfound->has_arg == 1) { if (d->optind < argc) d->optarg = argv[d->optind++]; else { if (print_errors) fprintf (stderr, _("%s: option '%s%s' requires an argument\n"), argv[0], prefix, pfound->name); d->optopt = pfound->val; return optstring[0] == ':' ? ':' : '?'; } } if (longind != NULL) *longind = option_index; if (pfound->flag) { *(pfound->flag) = pfound->val; return 0; } return pfound->val; } /* Initialize internal data upon the first call to getopt. */ static const char * _getopt_initialize (int argc _GL_UNUSED, char **argv _GL_UNUSED, const char *optstring, struct _getopt_data *d, int posixly_correct) { /* Start processing options with ARGV-element 1 (since ARGV-element 0 is the program name); the sequence of previously skipped non-option ARGV-elements is empty. */ if (d->optind == 0) d->optind = 1; d->__first_nonopt = d->__last_nonopt = d->optind; d->__nextchar = NULL; /* Determine how to handle the ordering of options and nonoptions. */ if (optstring[0] == '-') { d->__ordering = RETURN_IN_ORDER; ++optstring; } else if (optstring[0] == '+') { d->__ordering = REQUIRE_ORDER; ++optstring; } else if (posixly_correct || !!getenv ("POSIXLY_CORRECT")) d->__ordering = REQUIRE_ORDER; else d->__ordering = PERMUTE; d->__initialized = 1; return optstring; } /* Scan elements of ARGV (whose length is ARGC) for option characters given in OPTSTRING. If an element of ARGV starts with '-', and is not exactly "-" or "--", then it is an option element. The characters of this element (aside from the initial '-') are option characters. If 'getopt' is called repeatedly, it returns successively each of the option characters from each of the option elements. If 'getopt' finds another option character, it returns that character, updating 'optind' and 'nextchar' so that the next call to 'getopt' can resume the scan with the following option character or ARGV-element. If there are no more option characters, 'getopt' returns -1. Then 'optind' is the index in ARGV of the first ARGV-element that is not an option. (The ARGV-elements have been permuted so that those that are not options now come last.) OPTSTRING is a string containing the legitimate option characters. If an option character is seen that is not listed in OPTSTRING, return '?' after printing an error message. If you set 'opterr' to zero, the error message is suppressed but we still return '?'. If a char in OPTSTRING is followed by a colon, that means it wants an arg, so the following text in the same ARGV-element, or the text of the following ARGV-element, is returned in 'optarg'. Two colons mean an option that wants an optional arg; if there is text in the current ARGV-element, it is returned in 'optarg', otherwise 'optarg' is set to zero. If OPTSTRING starts with '-' or '+', it requests different methods of handling the non-option ARGV-elements. See the comments about RETURN_IN_ORDER and REQUIRE_ORDER, above. Long-named options begin with '--' instead of '-'. Their names may be abbreviated as long as the abbreviation is unique or is an exact match for some defined option. If they have an argument, it follows the option name in the same ARGV-element, separated from the option name by a '=', or else the in next ARGV-element. When 'getopt' finds a long-named option, it returns 0 if that option's 'flag' field is nonzero, the value of the option's 'val' field if the 'flag' field is zero. The elements of ARGV aren't really const, because we permute them. But we pretend they're const in the prototype to be compatible with other systems. LONGOPTS is a vector of 'struct option' terminated by an element containing a name which is zero. LONGIND returns the index in LONGOPT of the long-named option found. It is only valid when a long-named option has been found by the most recent call. If LONG_ONLY is nonzero, '-' as well as '--' can introduce long-named options. */ int _getopt_internal_r (int argc, char **argv, const char *optstring, const struct option *longopts, int *longind, int long_only, struct _getopt_data *d, int posixly_correct) { int print_errors = d->opterr; if (argc < 1) return -1; d->optarg = NULL; if (d->optind == 0 || !d->__initialized) optstring = _getopt_initialize (argc, argv, optstring, d, posixly_correct); else if (optstring[0] == '-' || optstring[0] == '+') optstring++; if (optstring[0] == ':') print_errors = 0; /* Test whether ARGV[optind] points to a non-option argument. */ #define NONOPTION_P (argv[d->optind][0] != '-' || argv[d->optind][1] == '\0') if (d->__nextchar == NULL || *d->__nextchar == '\0') { /* Advance to the next ARGV-element. */ /* Give FIRST_NONOPT & LAST_NONOPT rational values if OPTIND has been moved back by the user (who may also have changed the arguments). */ if (d->__last_nonopt > d->optind) d->__last_nonopt = d->optind; if (d->__first_nonopt > d->optind) d->__first_nonopt = d->optind; if (d->__ordering == PERMUTE) { /* If we have just processed some options following some non-options, exchange them so that the options come first. */ if (d->__first_nonopt != d->__last_nonopt && d->__last_nonopt != d->optind) exchange (argv, d); else if (d->__last_nonopt != d->optind) d->__first_nonopt = d->optind; /* Skip any additional non-options and extend the range of non-options previously skipped. */ while (d->optind < argc && NONOPTION_P) d->optind++; d->__last_nonopt = d->optind; } /* The special ARGV-element '--' means premature end of options. Skip it like a null option, then exchange with previous non-options as if it were an option, then skip everything else like a non-option. */ if (d->optind != argc && !strcmp (argv[d->optind], "--")) { d->optind++; if (d->__first_nonopt != d->__last_nonopt && d->__last_nonopt != d->optind) exchange (argv, d); else if (d->__first_nonopt == d->__last_nonopt) d->__first_nonopt = d->optind; d->__last_nonopt = argc; d->optind = argc; } /* If we have done all the ARGV-elements, stop the scan and back over any non-options that we skipped and permuted. */ if (d->optind == argc) { /* Set the next-arg-index to point at the non-options that we previously skipped, so the caller will digest them. */ if (d->__first_nonopt != d->__last_nonopt) d->optind = d->__first_nonopt; return -1; } /* If we have come to a non-option and did not permute it, either stop the scan or describe it to the caller and pass it by. */ if (NONOPTION_P) { if (d->__ordering == REQUIRE_ORDER) return -1; d->optarg = argv[d->optind++]; return 1; } /* We have found another option-ARGV-element. Check whether it might be a long option. */ if (longopts) { if (argv[d->optind][1] == '-') { /* "--foo" is always a long option. The special option "--" was handled above. */ d->__nextchar = argv[d->optind] + 2; return process_long_option (argc, argv, optstring, longopts, longind, long_only, d, print_errors, "--"); } /* If long_only and the ARGV-element has the form "-f", where f is a valid short option, don't consider it an abbreviated form of a long option that starts with f. Otherwise there would be no way to give the -f short option. On the other hand, if there's a long option "fubar" and the ARGV-element is "-fu", do consider that an abbreviation of the long option, just like "--fu", and not "-f" with arg "u". This distinction seems to be the most useful approach. */ if (long_only && (argv[d->optind][2] || !strchr (optstring, argv[d->optind][1]))) { int code; d->__nextchar = argv[d->optind] + 1; code = process_long_option (argc, argv, optstring, longopts, longind, long_only, d, print_errors, "-"); if (code != -1) return code; } } /* It is not a long option. Skip the initial punctuation. */ d->__nextchar = argv[d->optind] + 1; } /* Look at and handle the next short option-character. */ { char c = *d->__nextchar++; const char *temp = strchr (optstring, c); /* Increment 'optind' when we start to process its last character. */ if (*d->__nextchar == '\0') ++d->optind; if (temp == NULL || c == ':' || c == ';') { if (print_errors) fprintf (stderr, _("%s: invalid option -- '%c'\n"), argv[0], c); d->optopt = c; return '?'; } /* Convenience. Treat POSIX -W foo same as long option --foo */ if (temp[0] == 'W' && temp[1] == ';' && longopts != NULL) { /* This is an option that requires an argument. */ if (*d->__nextchar != '\0') d->optarg = d->__nextchar; else if (d->optind == argc) { if (print_errors) fprintf (stderr, _("%s: option requires an argument -- '%c'\n"), argv[0], c); d->optopt = c; if (optstring[0] == ':') c = ':'; else c = '?'; return c; } else d->optarg = argv[d->optind]; d->__nextchar = d->optarg; d->optarg = NULL; return process_long_option (argc, argv, optstring, longopts, longind, 0 /* long_only */, d, print_errors, "-W "); } if (temp[1] == ':') { if (temp[2] == ':') { /* This is an option that accepts an argument optionally. */ if (*d->__nextchar != '\0') { d->optarg = d->__nextchar; d->optind++; } else d->optarg = NULL; d->__nextchar = NULL; } else { /* This is an option that requires an argument. */ if (*d->__nextchar != '\0') { d->optarg = d->__nextchar; /* If we end this ARGV-element by taking the rest as an arg, we must advance to the next element now. */ d->optind++; } else if (d->optind == argc) { if (print_errors) fprintf (stderr, _("%s: option requires an argument -- '%c'\n"), argv[0], c); d->optopt = c; if (optstring[0] == ':') c = ':'; else c = '?'; } else /* We already incremented 'optind' once; increment it again when taking next ARGV-elt as argument. */ d->optarg = argv[d->optind++]; d->__nextchar = NULL; } } return c; } } int _getopt_internal (int argc, char **argv, const char *optstring, const struct option *longopts, int *longind, int long_only, int posixly_correct) { int result; getopt_data.optind = optind; getopt_data.opterr = opterr; result = _getopt_internal_r (argc, argv, optstring, longopts, longind, long_only, &getopt_data, posixly_correct); optind = getopt_data.optind; optarg = getopt_data.optarg; optopt = getopt_data.optopt; return result; } /* glibc gets a LSB-compliant getopt and a POSIX-complaint __posix_getopt. Standalone applications just get a POSIX-compliant getopt. POSIX and LSB both require these functions to take 'char *const *argv' even though this is incorrect (because of the permutation). */ #define GETOPT_ENTRY(NAME, POSIXLY_CORRECT) \ int \ NAME (int argc, char *const *argv, const char *optstring) \ { \ return _getopt_internal (argc, (char **)argv, optstring, \ 0, 0, 0, POSIXLY_CORRECT); \ } #ifdef _LIBC GETOPT_ENTRY(getopt, 0) GETOPT_ENTRY(__posix_getopt, 1) #else GETOPT_ENTRY(getopt, 1) #endif #ifdef TEST /* Compile with -DTEST to make an executable for use in testing the above definition of 'getopt'. */ int main (int argc, char **argv) { int c; int digit_optind = 0; while (1) { int this_option_optind = optind ? optind : 1; c = getopt (argc, argv, "abc:d:0123456789"); if (c == -1) break; switch (c) { case '0': case '1': case '2': case '3': case '4': case '5': case '6': case '7': case '8': case '9': if (digit_optind != 0 && digit_optind != this_option_optind) printf ("digits occur in two different argv-elements.\n"); digit_optind = this_option_optind; printf ("option %c\n", c); break; case 'a': printf ("option a\n"); break; case 'b': printf ("option b\n"); break; case 'c': printf ("option c with value '%s'\n", optarg); break; case '?': break; default: printf ("?? getopt returned character code 0%o ??\n", c); } } if (optind < argc) { printf ("non-option ARGV-elements: "); while (optind < argc) printf ("%s ", argv[optind++]); printf ("\n"); } exit (0); } #endif /* TEST */ gnuastro-0.5/bootstrapped/lib/getline.c0000644000175000017500000000166713217200021015206 00000000000000/* getline.c --- Implementation of replacement getline function. Copyright (C) 2005-2007, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Simon Josefsson. */ #include #include ssize_t getline (char **lineptr, size_t *n, FILE *stream) { return getdelim (lineptr, n, '\n', stream); } gnuastro-0.5/bootstrapped/lib/getdelim.c0000644000175000017500000000754113217200021015346 00000000000000/* getdelim.c --- Implementation of replacement getdelim function. Copyright (C) 1994, 1996-1998, 2001, 2003, 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Ported from glibc by Simon Josefsson. */ /* Don't use __attribute__ __nonnull__ in this compilation unit. Otherwise gcc optimizes away the lineptr == NULL || n == NULL || fp == NULL tests below. */ #define _GL_ARG_NONNULL(params) #include #include #include #include #include #include #ifndef SSIZE_MAX # define SSIZE_MAX ((ssize_t) (SIZE_MAX / 2)) #endif #if USE_UNLOCKED_IO # include "unlocked-io.h" # define getc_maybe_unlocked(fp) getc(fp) #elif !HAVE_FLOCKFILE || !HAVE_FUNLOCKFILE || !HAVE_DECL_GETC_UNLOCKED # undef flockfile # undef funlockfile # define flockfile(x) ((void) 0) # define funlockfile(x) ((void) 0) # define getc_maybe_unlocked(fp) getc(fp) #else # define getc_maybe_unlocked(fp) getc_unlocked(fp) #endif static void alloc_failed (void) { #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Avoid errno problem without using the realloc module; see: https://lists.gnu.org/r/bug-gnulib/2016-08/msg00025.html */ errno = ENOMEM; #endif } /* Read up to (and including) a DELIMITER from FP into *LINEPTR (and NUL-terminate it). *LINEPTR is a pointer returned from malloc (or NULL), pointing to *N characters of space. It is realloc'ed as necessary. Returns the number of characters read (not including the null terminator), or -1 on error or EOF. */ ssize_t getdelim (char **lineptr, size_t *n, int delimiter, FILE *fp) { ssize_t result; size_t cur_len = 0; if (lineptr == NULL || n == NULL || fp == NULL) { errno = EINVAL; return -1; } flockfile (fp); if (*lineptr == NULL || *n == 0) { char *new_lineptr; *n = 120; new_lineptr = (char *) realloc (*lineptr, *n); if (new_lineptr == NULL) { alloc_failed (); result = -1; goto unlock_return; } *lineptr = new_lineptr; } for (;;) { int i; i = getc_maybe_unlocked (fp); if (i == EOF) { result = -1; break; } /* Make enough space for len+1 (for final NUL) bytes. */ if (cur_len + 1 >= *n) { size_t needed_max = SSIZE_MAX < SIZE_MAX ? (size_t) SSIZE_MAX + 1 : SIZE_MAX; size_t needed = 2 * *n + 1; /* Be generous. */ char *new_lineptr; if (needed_max < needed) needed = needed_max; if (cur_len + 1 >= needed) { result = -1; errno = EOVERFLOW; goto unlock_return; } new_lineptr = (char *) realloc (*lineptr, needed); if (new_lineptr == NULL) { alloc_failed (); result = -1; goto unlock_return; } *lineptr = new_lineptr; *n = needed; } (*lineptr)[cur_len] = i; cur_len++; if (i == delimiter) break; } (*lineptr)[cur_len] = '\0'; result = cur_len ? cur_len : result; unlock_return: funlockfile (fp); /* doesn't set errno */ return result; } gnuastro-0.5/bootstrapped/lib/itold.c0000644000175000017500000000201113217200021014652 00000000000000/* Replacement for 'int' to 'long double' conversion routine. Copyright (C) 2011-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include void _Qp_itoq (long double *result, int a) { /* Convert from 'int' to 'double', then from 'double' to 'long double'. */ *result = (double) a; } gnuastro-0.5/bootstrapped/lib/float.c0000644000175000017500000000250513217200021014654 00000000000000/* Auxiliary definitions for . Copyright (C) 2011-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2011. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #if (defined _ARCH_PPC || defined _POWER) && (defined _AIX || defined __linux__) && (LDBL_MANT_DIG == 106) && defined __GNUC__ const union gl_long_double_union gl_LDBL_MAX = { { DBL_MAX, DBL_MAX / (double)134217728UL / (double)134217728UL } }; #elif defined __i386__ const union gl_long_double_union gl_LDBL_MAX = { { 0xFFFFFFFF, 0xFFFFFFFF, 32766 } }; #else /* This declaration is solely to ensure that after preprocessing this file is never empty. */ typedef int dummy; #endif gnuastro-0.5/bootstrapped/lib/error.c0000644000175000017500000002476313217200021014712 00000000000000/* Error handler for noninteractive utilities Copyright (C) 1990-1998, 2000-2007, 2009-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by David MacKenzie . */ #if !_LIBC # include #endif #include "error.h" #include #include #include #include #if !_LIBC && ENABLE_NLS # include "gettext.h" # define _(msgid) gettext (msgid) #endif #ifdef _LIBC # include # include # include # include # define mbsrtowcs __mbsrtowcs # define USE_UNLOCKED_IO 0 # define _GL_ATTRIBUTE_FORMAT_PRINTF(a, b) # define _GL_ARG_NONNULL(a) #else # include "getprogname.h" #endif #if USE_UNLOCKED_IO # include "unlocked-io.h" #endif #ifndef _ # define _(String) String #endif /* If NULL, error will flush stdout, then print on stderr the program name, a colon and a space. Otherwise, error will call this function without parameters instead. */ void (*error_print_progname) (void); /* This variable is incremented each time 'error' is called. */ unsigned int error_message_count; #ifdef _LIBC /* In the GNU C library, there is a predefined variable for this. */ # define program_name program_invocation_name # include # include # include /* In GNU libc we want do not want to use the common name 'error' directly. Instead make it a weak alias. */ extern void __error (int status, int errnum, const char *message, ...) __attribute__ ((__format__ (__printf__, 3, 4))); extern void __error_at_line (int status, int errnum, const char *file_name, unsigned int line_number, const char *message, ...) __attribute__ ((__format__ (__printf__, 5, 6))); # define error __error # define error_at_line __error_at_line # include # define fflush(s) _IO_fflush (s) # undef putc # define putc(c, fp) _IO_putc (c, fp) # include #else /* not _LIBC */ # include # include # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Get declarations of the native Windows API functions. */ # define WIN32_LEAN_AND_MEAN # include /* Get _get_osfhandle. */ # if GNULIB_MSVC_NOTHROW # include "msvc-nothrow.h" # else # include # endif # endif /* The gnulib override of fcntl is not needed in this file. */ # undef fcntl # if !(GNULIB_STRERROR_R_POSIX || HAVE_DECL_STRERROR_R) # ifndef HAVE_DECL_STRERROR_R "this configure-time declaration test was not run" # endif # if STRERROR_R_CHAR_P char *strerror_r (int errnum, char *buf, size_t buflen); # else int strerror_r (int errnum, char *buf, size_t buflen); # endif # endif #define program_name getprogname () # if GNULIB_STRERROR_R_POSIX || HAVE_STRERROR_R || defined strerror_r # define __strerror_r strerror_r # endif /* GNULIB_STRERROR_R_POSIX || HAVE_STRERROR_R || defined strerror_r */ #endif /* not _LIBC */ #if !_LIBC /* Return non-zero if FD is open. */ static int is_open (int fd) { # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* On native Windows: The initial state of unassigned standard file descriptors is that they are open but point to an INVALID_HANDLE_VALUE. There is no fcntl, and the gnulib replacement fcntl does not support F_GETFL. */ return (HANDLE) _get_osfhandle (fd) != INVALID_HANDLE_VALUE; # else # ifndef F_GETFL # error Please port fcntl to your platform # endif return 0 <= fcntl (fd, F_GETFL); # endif } #endif static void flush_stdout (void) { #if !_LIBC int stdout_fd; # if GNULIB_FREOPEN_SAFER /* Use of gnulib's freopen-safer module normally ensures that fileno (stdout) == 1 whenever stdout is open. */ stdout_fd = STDOUT_FILENO; # else /* POSIX states that fileno (stdout) after fclose is unspecified. But in practice it is not a problem, because stdout is statically allocated and the fd of a FILE stream is stored as a field in its allocated memory. */ stdout_fd = fileno (stdout); # endif /* POSIX states that fflush (stdout) after fclose is unspecified; it is safe in glibc, but not on all other platforms. fflush (NULL) is always defined, but too draconian. */ if (0 <= stdout_fd && is_open (stdout_fd)) #endif fflush (stdout); } static void print_errno_message (int errnum) { char const *s; #if _LIBC || GNULIB_STRERROR_R_POSIX || defined HAVE_STRERROR_R char errbuf[1024]; # if _LIBC || (!GNULIB_STRERROR_R_POSIX && STRERROR_R_CHAR_P) s = __strerror_r (errnum, errbuf, sizeof errbuf); # else if (__strerror_r (errnum, errbuf, sizeof errbuf) == 0) s = errbuf; else s = 0; # endif #else s = strerror (errnum); #endif #if !_LIBC if (! s) s = _("Unknown system error"); #endif #if _LIBC __fxprintf (NULL, ": %s", s); #else fprintf (stderr, ": %s", s); #endif } static void _GL_ATTRIBUTE_FORMAT_PRINTF (3, 0) _GL_ARG_NONNULL ((3)) error_tail (int status, int errnum, const char *message, va_list args) { #if _LIBC if (_IO_fwide (stderr, 0) > 0) { size_t len = strlen (message) + 1; wchar_t *wmessage = NULL; mbstate_t st; size_t res; const char *tmp; bool use_malloc = false; while (1) { if (__libc_use_alloca (len * sizeof (wchar_t))) wmessage = (wchar_t *) alloca (len * sizeof (wchar_t)); else { if (!use_malloc) wmessage = NULL; wchar_t *p = (wchar_t *) realloc (wmessage, len * sizeof (wchar_t)); if (p == NULL) { free (wmessage); fputws_unlocked (L"out of memory\n", stderr); return; } wmessage = p; use_malloc = true; } memset (&st, '\0', sizeof (st)); tmp = message; res = mbsrtowcs (wmessage, &tmp, len, &st); if (res != len) break; if (__builtin_expect (len >= SIZE_MAX / sizeof (wchar_t) / 2, 0)) { /* This really should not happen if everything is fine. */ res = (size_t) -1; break; } len *= 2; } if (res == (size_t) -1) { /* The string cannot be converted. */ if (use_malloc) { free (wmessage); use_malloc = false; } wmessage = (wchar_t *) L"???"; } __vfwprintf (stderr, wmessage, args); if (use_malloc) free (wmessage); } else #endif vfprintf (stderr, message, args); ++error_message_count; if (errnum) print_errno_message (errnum); #if _LIBC __fxprintf (NULL, "\n"); #else putc ('\n', stderr); #endif fflush (stderr); if (status) exit (status); } /* Print the program name and error message MESSAGE, which is a printf-style format string with optional args. If ERRNUM is nonzero, print its corresponding system error message. Exit with status STATUS if it is nonzero. */ void error (int status, int errnum, const char *message, ...) { va_list args; #if defined _LIBC && defined __libc_ptf_call /* We do not want this call to be cut short by a thread cancellation. Therefore disable cancellation for now. */ int state = PTHREAD_CANCEL_ENABLE; __libc_ptf_call (pthread_setcancelstate, (PTHREAD_CANCEL_DISABLE, &state), 0); #endif flush_stdout (); #ifdef _LIBC _IO_flockfile (stderr); #endif if (error_print_progname) (*error_print_progname) (); else { #if _LIBC __fxprintf (NULL, "%s: ", program_name); #else fprintf (stderr, "%s: ", program_name); #endif } va_start (args, message); error_tail (status, errnum, message, args); va_end (args); #ifdef _LIBC _IO_funlockfile (stderr); # ifdef __libc_ptf_call __libc_ptf_call (pthread_setcancelstate, (state, NULL), 0); # endif #endif } /* Sometimes we want to have at most one error per line. This variable controls whether this mode is selected or not. */ int error_one_per_line; void error_at_line (int status, int errnum, const char *file_name, unsigned int line_number, const char *message, ...) { va_list args; if (error_one_per_line) { static const char *old_file_name; static unsigned int old_line_number; if (old_line_number == line_number && (file_name == old_file_name || (old_file_name != NULL && file_name != NULL && strcmp (old_file_name, file_name) == 0))) /* Simply return and print nothing. */ return; old_file_name = file_name; old_line_number = line_number; } #if defined _LIBC && defined __libc_ptf_call /* We do not want this call to be cut short by a thread cancellation. Therefore disable cancellation for now. */ int state = PTHREAD_CANCEL_ENABLE; __libc_ptf_call (pthread_setcancelstate, (PTHREAD_CANCEL_DISABLE, &state), 0); #endif flush_stdout (); #ifdef _LIBC _IO_flockfile (stderr); #endif if (error_print_progname) (*error_print_progname) (); else { #if _LIBC __fxprintf (NULL, "%s:", program_name); #else fprintf (stderr, "%s:", program_name); #endif } #if _LIBC __fxprintf (NULL, file_name != NULL ? "%s:%u: " : " ", file_name, line_number); #else fprintf (stderr, file_name != NULL ? "%s:%u: " : " ", file_name, line_number); #endif va_start (args, message); error_tail (status, errnum, message, args); va_end (args); #ifdef _LIBC _IO_funlockfile (stderr); # ifdef __libc_ptf_call __libc_ptf_call (pthread_setcancelstate, (state, NULL), 0); # endif #endif } #ifdef _LIBC /* Make the weak alias. */ # undef error # undef error_at_line weak_alias (__error, error) weak_alias (__error_at_line, error_at_line) #endif gnuastro-0.5/bootstrapped/lib/btowc.c0000644000175000017500000000211013217200020014654 00000000000000/* Convert unibyte character to wide character. Copyright (C) 2008, 2010-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2008. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include #include wint_t btowc (int c) { if (c != EOF) { char buf[1]; wchar_t wc; buf[0] = c; if (mbtowc (&wc, buf, 1) >= 0) return wc; } return WEOF; } gnuastro-0.5/bootstrapped/lib/xsize.c0000644000175000017500000000011613217200022014706 00000000000000#include #define XSIZE_INLINE _GL_EXTERN_INLINE #include "xsize.h" gnuastro-0.5/bootstrapped/lib/xsize.h0000644000175000017500000000705713217200022014726 00000000000000/* xsize.h -- Checked size_t computations. Copyright (C) 2003, 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _XSIZE_H #define _XSIZE_H /* Get size_t. */ #include /* Get SIZE_MAX. */ #include #if HAVE_STDINT_H # include #endif #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef XSIZE_INLINE # define XSIZE_INLINE _GL_INLINE #endif /* The size of memory objects is often computed through expressions of type size_t. Example: void* p = malloc (header_size + n * element_size). These computations can lead to overflow. When this happens, malloc() returns a piece of memory that is way too small, and the program then crashes while attempting to fill the memory. To avoid this, the functions and macros in this file check for overflow. The convention is that SIZE_MAX represents overflow. malloc (SIZE_MAX) is not guaranteed to fail -- think of a malloc implementation that uses mmap --, it's recommended to use size_overflow_p() or size_in_bounds_p() before invoking malloc(). The example thus becomes: size_t size = xsum (header_size, xtimes (n, element_size)); void *p = (size_in_bounds_p (size) ? malloc (size) : NULL); */ /* Convert an arbitrary value >= 0 to type size_t. */ #define xcast_size_t(N) \ ((N) <= SIZE_MAX ? (size_t) (N) : SIZE_MAX) /* Sum of two sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xsum (size_t size1, size_t size2) { size_t sum = size1 + size2; return (sum >= size1 ? sum : SIZE_MAX); } /* Sum of three sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xsum3 (size_t size1, size_t size2, size_t size3) { return xsum (xsum (size1, size2), size3); } /* Sum of four sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xsum4 (size_t size1, size_t size2, size_t size3, size_t size4) { return xsum (xsum (xsum (size1, size2), size3), size4); } /* Maximum of two sizes, with overflow check. */ XSIZE_INLINE size_t #if __GNUC__ >= 3 __attribute__ ((__pure__)) #endif xmax (size_t size1, size_t size2) { /* No explicit check is needed here, because for any n: max (SIZE_MAX, n) == SIZE_MAX and max (n, SIZE_MAX) == SIZE_MAX. */ return (size1 >= size2 ? size1 : size2); } /* Multiplication of a count with an element size, with overflow check. The count must be >= 0 and the element size must be > 0. This is a macro, not a function, so that it works correctly even when N is of a wider type and N > SIZE_MAX. */ #define xtimes(N, ELSIZE) \ ((N) <= SIZE_MAX / (ELSIZE) ? (size_t) (N) * (ELSIZE) : SIZE_MAX) /* Check for overflow. */ #define size_overflow_p(SIZE) \ ((SIZE) == SIZE_MAX) /* Check against overflow. */ #define size_in_bounds_p(SIZE) \ ((SIZE) != SIZE_MAX) _GL_INLINE_HEADER_END #endif /* _XSIZE_H */ gnuastro-0.5/bootstrapped/lib/wctype-h.c0000644000175000017500000000023313217200022015304 00000000000000/* Normally this would be wctype.c, but that name's already taken. */ #include #define _GL_WCTYPE_INLINE _GL_EXTERN_INLINE #include "wctype.h" gnuastro-0.5/bootstrapped/lib/unistd.c0000644000175000017500000000014713217200021015055 00000000000000#include #define _GL_UNISTD_INLINE _GL_EXTERN_INLINE #include "unistd.h" typedef int dummy; gnuastro-0.5/bootstrapped/lib/strnlen1.c0000644000175000017500000000236613217200021015322 00000000000000/* Find the length of STRING + 1, but scan at most MAXLEN bytes. Copyright (C) 2005-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include "strnlen1.h" #include /* Find the length of STRING + 1, but scan at most MAXLEN bytes. If no '\0' terminator is found in that many characters, return MAXLEN. */ /* This is the same as strnlen (string, maxlen - 1) + 1. */ size_t strnlen1 (const char *string, size_t maxlen) { const char *end = (const char *) memchr (string, '\0', maxlen); if (end != NULL) return end - string + 1; else return maxlen; } gnuastro-0.5/bootstrapped/lib/strnlen1.h0000644000175000017500000000231013217200021015314 00000000000000/* Find the length of STRING + 1, but scan at most MAXLEN bytes. Copyright (C) 2005, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _STRNLEN1_H #define _STRNLEN1_H #include #ifdef __cplusplus extern "C" { #endif /* Find the length of STRING + 1, but scan at most MAXLEN bytes. If no '\0' terminator is found in that many characters, return MAXLEN. */ /* This is the same as strnlen (string, maxlen - 1) + 1. */ extern size_t strnlen1 (const char *string, size_t maxlen) _GL_ATTRIBUTE_PURE; #ifdef __cplusplus } #endif #endif /* _STRNLEN1_H */ gnuastro-0.5/bootstrapped/lib/size_max.h0000644000175000017500000000221213217200021015366 00000000000000/* size_max.h -- declare SIZE_MAX through system headers Copyright (C) 2005-2006, 2009-2017 Free Software Foundation, Inc. Written by Simon Josefsson. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef GNULIB_SIZE_MAX_H #define GNULIB_SIZE_MAX_H /* Get SIZE_MAX declaration on systems like Solaris 7/8/9. */ # include /* Get SIZE_MAX declaration on systems like glibc 2. */ # if HAVE_STDINT_H # include # endif /* On systems where these include files don't define it, SIZE_MAX is defined in config.h. */ #endif /* GNULIB_SIZE_MAX_H */ gnuastro-0.5/bootstrapped/lib/nproc.c0000644000175000017500000002525513217200021014677 00000000000000/* Detect the number of processors. Copyright (C) 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Glen Lenker and Bruno Haible. */ #include #include "nproc.h" #include #include #include #if HAVE_PTHREAD_GETAFFINITY_NP && 0 # include # include #endif #if HAVE_SCHED_GETAFFINITY_LIKE_GLIBC || HAVE_SCHED_GETAFFINITY_NP # include #endif #include #if HAVE_SYS_PSTAT_H # include #endif #if HAVE_SYS_SYSMP_H # include #endif #if HAVE_SYS_PARAM_H # include #endif #if HAVE_SYS_SYSCTL_H # include #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include #endif #include "c-ctype.h" #include "minmax.h" #define ARRAY_SIZE(a) (sizeof (a) / sizeof ((a)[0])) /* Return the number of processors available to the current process, based on a modern system call that returns the "affinity" between the current process and each CPU. Return 0 if unknown or if such a system call does not exist. */ static unsigned long num_processors_via_affinity_mask (void) { /* glibc >= 2.3.3 with NPTL and NetBSD 5 have pthread_getaffinity_np, but with different APIs. Also it requires linking with -lpthread. Therefore this code is not enabled. glibc >= 2.3.4 has sched_getaffinity whereas NetBSD 5 has sched_getaffinity_np. */ #if HAVE_PTHREAD_GETAFFINITY_NP && defined __GLIBC__ && 0 { cpu_set_t set; if (pthread_getaffinity_np (pthread_self (), sizeof (set), &set) == 0) { unsigned long count; # ifdef CPU_COUNT /* glibc >= 2.6 has the CPU_COUNT macro. */ count = CPU_COUNT (&set); # else size_t i; count = 0; for (i = 0; i < CPU_SETSIZE; i++) if (CPU_ISSET (i, &set)) count++; # endif if (count > 0) return count; } } #elif HAVE_PTHREAD_GETAFFINITY_NP && defined __NetBSD__ && 0 { cpuset_t *set; set = cpuset_create (); if (set != NULL) { unsigned long count = 0; if (pthread_getaffinity_np (pthread_self (), cpuset_size (set), set) == 0) { cpuid_t i; for (i = 0;; i++) { int ret = cpuset_isset (i, set); if (ret < 0) break; if (ret > 0) count++; } } cpuset_destroy (set); if (count > 0) return count; } } #elif HAVE_SCHED_GETAFFINITY_LIKE_GLIBC /* glibc >= 2.3.4 */ { cpu_set_t set; if (sched_getaffinity (0, sizeof (set), &set) == 0) { unsigned long count; # ifdef CPU_COUNT /* glibc >= 2.6 has the CPU_COUNT macro. */ count = CPU_COUNT (&set); # else size_t i; count = 0; for (i = 0; i < CPU_SETSIZE; i++) if (CPU_ISSET (i, &set)) count++; # endif if (count > 0) return count; } } #elif HAVE_SCHED_GETAFFINITY_NP /* NetBSD >= 5 */ { cpuset_t *set; set = cpuset_create (); if (set != NULL) { unsigned long count = 0; if (sched_getaffinity_np (getpid (), cpuset_size (set), set) == 0) { cpuid_t i; for (i = 0;; i++) { int ret = cpuset_isset (i, set); if (ret < 0) break; if (ret > 0) count++; } } cpuset_destroy (set); if (count > 0) return count; } } #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { /* This works on native Windows platforms. */ DWORD_PTR process_mask; DWORD_PTR system_mask; if (GetProcessAffinityMask (GetCurrentProcess (), &process_mask, &system_mask)) { DWORD_PTR mask = process_mask; unsigned long count = 0; for (; mask != 0; mask = mask >> 1) if (mask & 1) count++; if (count > 0) return count; } } #endif return 0; } /* Return the total number of processors. Here QUERY must be one of NPROC_ALL, NPROC_CURRENT. The result is guaranteed to be at least 1. */ static unsigned long int num_processors_ignoring_omp (enum nproc_query query) { /* On systems with a modern affinity mask system call, we have sysconf (_SC_NPROCESSORS_CONF) >= sysconf (_SC_NPROCESSORS_ONLN) >= num_processors_via_affinity_mask () The first number is the number of CPUs configured in the system. The second number is the number of CPUs available to the scheduler. The third number is the number of CPUs available to the current process. Note! On Linux systems with glibc, the first and second number come from the /sys and /proc file systems (see glibc/sysdeps/unix/sysv/linux/getsysstats.c). In some situations these file systems are not mounted, and the sysconf call returns 1, which does not reflect the reality. */ if (query == NPROC_CURRENT) { /* Try the modern affinity mask system call. */ { unsigned long nprocs = num_processors_via_affinity_mask (); if (nprocs > 0) return nprocs; } #if defined _SC_NPROCESSORS_ONLN { /* This works on glibc, Mac OS X 10.5, FreeBSD, AIX, OSF/1, Solaris, Cygwin, Haiku. */ long int nprocs = sysconf (_SC_NPROCESSORS_ONLN); if (nprocs > 0) return nprocs; } #endif } else /* query == NPROC_ALL */ { #if defined _SC_NPROCESSORS_CONF { /* This works on glibc, Mac OS X 10.5, FreeBSD, AIX, OSF/1, Solaris, Cygwin, Haiku. */ long int nprocs = sysconf (_SC_NPROCESSORS_CONF); # if __GLIBC__ >= 2 && defined __linux__ /* On Linux systems with glibc, this information comes from the /sys and /proc file systems (see glibc/sysdeps/unix/sysv/linux/getsysstats.c). In some situations these file systems are not mounted, and the sysconf call returns 1. But we wish to guarantee that num_processors (NPROC_ALL) >= num_processors (NPROC_CURRENT). */ if (nprocs == 1) { unsigned long nprocs_current = num_processors_via_affinity_mask (); if (nprocs_current > 0) nprocs = nprocs_current; } # endif if (nprocs > 0) return nprocs; } #endif } #if HAVE_PSTAT_GETDYNAMIC { /* This works on HP-UX. */ struct pst_dynamic psd; if (pstat_getdynamic (&psd, sizeof psd, 1, 0) >= 0) { /* The field psd_proc_cnt contains the number of active processors. In newer releases of HP-UX 11, the field psd_max_proc_cnt includes deactivated processors. */ if (query == NPROC_CURRENT) { if (psd.psd_proc_cnt > 0) return psd.psd_proc_cnt; } else { if (psd.psd_max_proc_cnt > 0) return psd.psd_max_proc_cnt; } } } #endif #if HAVE_SYSMP && defined MP_NAPROCS && defined MP_NPROCS { /* This works on IRIX. */ /* MP_NPROCS yields the number of installed processors. MP_NAPROCS yields the number of processors available to unprivileged processes. */ int nprocs = sysmp (query == NPROC_CURRENT && getpid () != 0 ? MP_NAPROCS : MP_NPROCS); if (nprocs > 0) return nprocs; } #endif /* Finally, as fallback, use the APIs that don't distinguish between NPROC_CURRENT and NPROC_ALL. */ #if HAVE_SYSCTL && defined HW_NCPU { /* This works on Mac OS X, FreeBSD, NetBSD, OpenBSD. */ int nprocs; size_t len = sizeof (nprocs); static int mib[2] = { CTL_HW, HW_NCPU }; if (sysctl (mib, ARRAY_SIZE (mib), &nprocs, &len, NULL, 0) == 0 && len == sizeof (nprocs) && 0 < nprocs) return nprocs; } #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ { /* This works on native Windows platforms. */ SYSTEM_INFO system_info; GetSystemInfo (&system_info); if (0 < system_info.dwNumberOfProcessors) return system_info.dwNumberOfProcessors; } #endif return 1; } /* Parse OMP environment variables without dependence on OMP. Return 0 for invalid values. */ static unsigned long int parse_omp_threads (char const* threads) { unsigned long int ret = 0; if (threads == NULL) return ret; /* The OpenMP spec says that the value assigned to the environment variables "may have leading and trailing white space". */ while (*threads != '\0' && c_isspace (*threads)) threads++; /* Convert it from positive decimal to 'unsigned long'. */ if (c_isdigit (*threads)) { char *endptr = NULL; unsigned long int value = strtoul (threads, &endptr, 10); if (endptr != NULL) { while (*endptr != '\0' && c_isspace (*endptr)) endptr++; if (*endptr == '\0') return value; /* Also accept the first value in a nesting level, since we can't determine the nesting level from env vars. */ else if (*endptr == ',') return value; } } return ret; } unsigned long int num_processors (enum nproc_query query) { unsigned long int omp_env_limit = ULONG_MAX; if (query == NPROC_CURRENT_OVERRIDABLE) { unsigned long int omp_env_threads; /* Honor the OpenMP environment variables, recognized also by all programs that are based on OpenMP. */ omp_env_threads = parse_omp_threads (getenv ("OMP_NUM_THREADS")); omp_env_limit = parse_omp_threads (getenv ("OMP_THREAD_LIMIT")); if (! omp_env_limit) omp_env_limit = ULONG_MAX; if (omp_env_threads) return MIN (omp_env_threads, omp_env_limit); query = NPROC_CURRENT; } /* Here query is one of NPROC_ALL, NPROC_CURRENT. */ { unsigned long nprocs = num_processors_ignoring_omp (query); return MIN (nprocs, omp_env_limit); } } gnuastro-0.5/bootstrapped/lib/minmax.h0000644000175000017500000000447113217200021015051 00000000000000/* MIN, MAX macros. Copyright (C) 1995, 1998, 2001, 2003, 2005, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _MINMAX_H #define _MINMAX_H /* Note: MIN, MAX are also defined in on some systems (glibc, IRIX, HP-UX, OSF/1). Therefore you might get warnings about MIN, MAX macro redefinitions on some systems; the workaround is to #include this file as the last one among the #include list. */ /* Before we define the following symbols we get the file since otherwise we get redefinitions on some systems if is included after this file. Likewise for . If more than one of these system headers define MIN and MAX, pick just one of the headers (because the definitions most likely are the same). */ #if HAVE_MINMAX_IN_LIMITS_H # include #elif HAVE_MINMAX_IN_SYS_PARAM_H # include #endif /* Note: MIN and MAX should be used with two arguments of the same type. They might not return the minimum and maximum of their two arguments, if the arguments have different types or have unusual floating-point values. For example, on a typical host with 32-bit 'int', 64-bit 'long long', and 64-bit IEEE 754 'double' types: MAX (-1, 2147483648) returns 4294967295. MAX (9007199254740992.0, 9007199254740993) returns 9007199254740992.0. MAX (NaN, 0.0) returns 0.0. MAX (+0.0, -0.0) returns -0.0. and in each case the answer is in some sense bogus. */ /* MAX(a,b) returns the maximum of A and B. */ #ifndef MAX # define MAX(a,b) ((a) > (b) ? (a) : (b)) #endif /* MIN(a,b) returns the minimum of A and B. */ #ifndef MIN # define MIN(a,b) ((a) < (b) ? (a) : (b)) #endif #endif /* _MINMAX_H */ gnuastro-0.5/bootstrapped/lib/mbuiter.c0000644000175000017500000000012213217200021015207 00000000000000#include #define MBUITER_INLINE _GL_EXTERN_INLINE #include "mbuiter.h" gnuastro-0.5/bootstrapped/lib/mbuiter.h0000644000175000017500000001752413217200021015232 00000000000000/* Iterating through multibyte strings: macros for multi-byte encodings. Copyright (C) 2001, 2005, 2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* Written by Bruno Haible . */ /* The macros in this file implement forward iteration through a multi-byte string, without knowing its length a-priori. With these macros, an iteration loop that looks like char *iter; for (iter = buf; *iter != '\0'; iter++) { do_something (*iter); } becomes mbui_iterator_t iter; for (mbui_init (iter, buf); mbui_avail (iter); mbui_advance (iter)) { do_something (mbui_cur_ptr (iter), mb_len (mbui_cur (iter))); } The benefit of these macros over plain use of mbrtowc is: - Handling of invalid multibyte sequences is possible without making the code more complicated, while still preserving the invalid multibyte sequences. Compared to mbiter.h, the macros here don't need to know the string's length a-priori. The downside is that at each step, the look-ahead that guards against overrunning the terminating '\0' is more expensive. The mbui_* macros are therefore suitable when there is a high probability that only the first few multibyte characters need to be inspected. Whereas the mbi_* macros are better if usually the iteration runs through the entire string. mbui_iterator_t is a type usable for variable declarations. mbui_init (iter, startptr) initializes the iterator, starting at startptr. mbui_avail (iter) returns true if there are more multibyte characters available before the end of string is reached. In this case, mbui_cur (iter) is initialized to the next multibyte character. mbui_advance (iter) advances the iterator by one multibyte character. mbui_cur (iter) returns the current multibyte character, of type mbchar_t. All the macros defined in mbchar.h can be used on it. mbui_cur_ptr (iter) return a pointer to the beginning of the current multibyte character. mbui_reloc (iter, ptrdiff) relocates iterator when the string is moved by ptrdiff bytes. mbui_copy (&destiter, &srciter) copies srciter to destiter. Here are the function prototypes of the macros. extern void mbui_init (mbui_iterator_t iter, const char *startptr); extern bool mbui_avail (mbui_iterator_t iter); extern void mbui_advance (mbui_iterator_t iter); extern mbchar_t mbui_cur (mbui_iterator_t iter); extern const char * mbui_cur_ptr (mbui_iterator_t iter); extern void mbui_reloc (mbui_iterator_t iter, ptrdiff_t ptrdiff); extern void mbui_copy (mbui_iterator_t *new, const mbui_iterator_t *old); */ #ifndef _MBUITER_H #define _MBUITER_H 1 #include #include #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.1 has a bug: and must be included before . */ #include #include #include #include "mbchar.h" #include "strnlen1.h" #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef MBUITER_INLINE # define MBUITER_INLINE _GL_INLINE #endif struct mbuiter_multi { bool in_shift; /* true if next byte may not be interpreted as ASCII */ mbstate_t state; /* if in_shift: current shift state */ bool next_done; /* true if mbui_avail has already filled the following */ struct mbchar cur; /* the current character: const char *cur.ptr pointer to current character The following are only valid after mbui_avail. size_t cur.bytes number of bytes of current character bool cur.wc_valid true if wc is a valid wide character wchar_t cur.wc if wc_valid: the current character */ }; MBUITER_INLINE void mbuiter_multi_next (struct mbuiter_multi *iter) { if (iter->next_done) return; if (iter->in_shift) goto with_shift; /* Handle most ASCII characters quickly, without calling mbrtowc(). */ if (is_basic (*iter->cur.ptr)) { /* These characters are part of the basic character set. ISO C 99 guarantees that their wide character code is identical to their char code. */ iter->cur.bytes = 1; iter->cur.wc = *iter->cur.ptr; iter->cur.wc_valid = true; } else { assert (mbsinit (&iter->state)); iter->in_shift = true; with_shift: iter->cur.bytes = mbrtowc (&iter->cur.wc, iter->cur.ptr, strnlen1 (iter->cur.ptr, MB_CUR_MAX), &iter->state); if (iter->cur.bytes == (size_t) -1) { /* An invalid multibyte sequence was encountered. */ iter->cur.bytes = 1; iter->cur.wc_valid = false; /* Whether to set iter->in_shift = false and reset iter->state or not is not very important; the string is bogus anyway. */ } else if (iter->cur.bytes == (size_t) -2) { /* An incomplete multibyte character at the end. */ iter->cur.bytes = strlen (iter->cur.ptr); iter->cur.wc_valid = false; /* Whether to set iter->in_shift = false and reset iter->state or not is not important; the string end is reached anyway. */ } else { if (iter->cur.bytes == 0) { /* A null wide character was encountered. */ iter->cur.bytes = 1; assert (*iter->cur.ptr == '\0'); assert (iter->cur.wc == 0); } iter->cur.wc_valid = true; /* When in the initial state, we can go back treating ASCII characters more quickly. */ if (mbsinit (&iter->state)) iter->in_shift = false; } } iter->next_done = true; } MBUITER_INLINE void mbuiter_multi_reloc (struct mbuiter_multi *iter, ptrdiff_t ptrdiff) { iter->cur.ptr += ptrdiff; } MBUITER_INLINE void mbuiter_multi_copy (struct mbuiter_multi *new_iter, const struct mbuiter_multi *old_iter) { if ((new_iter->in_shift = old_iter->in_shift)) memcpy (&new_iter->state, &old_iter->state, sizeof (mbstate_t)); else memset (&new_iter->state, 0, sizeof (mbstate_t)); new_iter->next_done = old_iter->next_done; mb_copy (&new_iter->cur, &old_iter->cur); } /* Iteration macros. */ typedef struct mbuiter_multi mbui_iterator_t; #define mbui_init(iter, startptr) \ ((iter).cur.ptr = (startptr), \ (iter).in_shift = false, memset (&(iter).state, '\0', sizeof (mbstate_t)), \ (iter).next_done = false) #define mbui_avail(iter) \ (mbuiter_multi_next (&(iter)), !mb_isnul ((iter).cur)) #define mbui_advance(iter) \ ((iter).cur.ptr += (iter).cur.bytes, (iter).next_done = false) /* Access to the current character. */ #define mbui_cur(iter) (iter).cur #define mbui_cur_ptr(iter) (iter).cur.ptr /* Relocation. */ #define mbui_reloc(iter, ptrdiff) mbuiter_multi_reloc (&iter, ptrdiff) /* Copying an iterator. */ #define mbui_copy mbuiter_multi_copy _GL_INLINE_HEADER_END #endif /* _MBUITER_H */ gnuastro-0.5/bootstrapped/lib/mbstok_r.c0000644000175000017500000000340713217200021015371 00000000000000/* Tokenizing a string. Copyright (C) 1999, 2002, 2006-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "mbuiter.h" char * mbstok_r (char *string, const char *delim, char **save_ptr) { if (MB_CUR_MAX > 1) { if (string == NULL) { string = *save_ptr; if (string == NULL) return NULL; /* reminder that end of token sequence has been reached */ } /* Skip leading delimiters. */ string += mbsspn (string, delim); /* Found a token? */ if (*string == '\0') { *save_ptr = NULL; return NULL; } /* Move past the token. */ { char *token_end = mbspbrk (string, delim); if (token_end != NULL) { /* NUL-terminate the token. */ *token_end = '\0'; *save_ptr = token_end + 1; } else *save_ptr = NULL; } return string; } else return strtok_r (string, delim, save_ptr); } gnuastro-0.5/bootstrapped/lib/mbsspn.c0000644000175000017500000000527613217200021015061 00000000000000/* Searching a string for a character outside a given set of characters. Copyright (C) 1999, 2002, 2006-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "mbuiter.h" /* Find the first occurrence in the character string STRING of any character not in the character string REJECT. Return the number of bytes from the beginning of the string to this occurrence, or to the end of the string if none exists. */ size_t mbsspn (const char *string, const char *reject) { /* Optimize two cases. */ if (reject[0] == '\0') return 0; if (reject[1] == '\0') { unsigned char uc = (unsigned char) reject[0]; if (MB_CUR_MAX > 1) { mbui_iterator_t iter; for (mbui_init (iter, string); mbui_avail (iter); mbui_advance (iter)) if (!(mb_len (mbui_cur (iter)) == 1 && (unsigned char) * mbui_cur_ptr (iter) == uc)) break; return mbui_cur_ptr (iter) - string; } else { const char *ptr; for (ptr = string; *ptr != '\0'; ptr++) if ((unsigned char) *ptr != uc) break; return ptr - string; } } /* General case. */ if (MB_CUR_MAX > 1) { mbui_iterator_t iter; for (mbui_init (iter, string); mbui_avail (iter); mbui_advance (iter)) { if (mb_len (mbui_cur (iter)) == 1) { if (mbschr (reject, * mbui_cur_ptr (iter)) == NULL) goto found; } else { mbui_iterator_t aiter; for (mbui_init (aiter, reject);; mbui_advance (aiter)) { if (!mbui_avail (aiter)) goto found; if (mb_equal (mbui_cur (aiter), mbui_cur (iter))) break; } } } found: return mbui_cur_ptr (iter) - string; } else return strspn (string, reject); } gnuastro-0.5/bootstrapped/lib/mbspbrk.c0000644000175000017500000000400313217200021015202 00000000000000/* Searching a string for a character among a given set of characters. Copyright (C) 1999, 2002, 2006-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "mbuiter.h" /* Find the first occurrence in the character string STRING of any character in the character string ACCEPT. Return the pointer to it, or NULL if none exists. */ char * mbspbrk (const char *string, const char *accept) { /* Optimize two cases. */ if (accept[0] == '\0') return NULL; if (accept[1] == '\0') return mbschr (string, accept[0]); /* General case. */ if (MB_CUR_MAX > 1) { mbui_iterator_t iter; for (mbui_init (iter, string); mbui_avail (iter); mbui_advance (iter)) { if (mb_len (mbui_cur (iter)) == 1) { if (mbschr (accept, * mbui_cur_ptr (iter))) return (char *) mbui_cur_ptr (iter); } else { mbui_iterator_t aiter; for (mbui_init (aiter, accept); mbui_avail (aiter); mbui_advance (aiter)) if (mb_equal (mbui_cur (aiter), mbui_cur (iter))) return (char *) mbui_cur_ptr (iter); } } return NULL; } else return strpbrk (string, accept); } gnuastro-0.5/bootstrapped/lib/mbschr.c0000644000175000017500000000336413217200021015031 00000000000000/* Searching a string for a character. Copyright (C) 2007-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2007. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include #include "mbuiter.h" /* Locate the first single-byte character C in the character string STRING, and return a pointer to it. Return NULL if C is not found in STRING. */ char * mbschr (const char *string, int c) { if (MB_CUR_MAX > 1 /* Optimization: We know that ASCII characters < 0x30 don't occur as part of multibyte characters longer than 1 byte. Hence, if c < 0x30, the faster unibyte loop can be used. */ && (unsigned char) c >= 0x30) { mbui_iterator_t iter; for (mbui_init (iter, string);; mbui_advance (iter)) { if (!mbui_avail (iter)) goto notfound; if (mb_len (mbui_cur (iter)) == 1 && (unsigned char) * mbui_cur_ptr (iter) == (unsigned char) c) break; } return (char *) mbui_cur_ptr (iter); notfound: return NULL; } else return strchr (string, c); } gnuastro-0.5/bootstrapped/lib/mbchar.c0000644000175000017500000000234113217200021015001 00000000000000/* Copyright (C) 2001, 2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #define MBCHAR_INLINE _GL_EXTERN_INLINE #include #include "mbchar.h" #if IS_BASIC_ASCII /* Bit table of characters in the ISO C "basic character set". */ const unsigned int is_basic_table [UCHAR_MAX / 32 + 1] = { 0x00001a00, /* '\t' '\v' '\f' */ 0xffffffef, /* ' '...'#' '%'...'?' */ 0xfffffffe, /* 'A'...'Z' '[' '\\' ']' '^' '_' */ 0x7ffffffe /* 'a'...'z' '{' '|' '}' '~' */ /* The remaining bits are 0. */ }; #endif /* IS_BASIC_ASCII */ gnuastro-0.5/bootstrapped/lib/math.c0000644000175000017500000000014313217200021014474 00000000000000#include #define _GL_MATH_INLINE _GL_EXTERN_INLINE #include "math.h" typedef int dummy; gnuastro-0.5/bootstrapped/lib/localcharset.c0000644000175000017500000005033313217200021016215 00000000000000/* Determine a canonical name for the current locale's character encoding. Copyright (C) 2000-2006, 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible . */ #include /* Specification. */ #include "localcharset.h" #include #include #include #include #include #if defined __APPLE__ && defined __MACH__ && HAVE_LANGINFO_CODESET # define DARWIN7 /* Darwin 7 or newer, i.e. Mac OS X 10.3 or newer */ #endif #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ # define WINDOWS_NATIVE # include #endif #if defined __EMX__ /* Assume EMX program runs on OS/2, even if compiled under DOS. */ # ifndef OS2 # define OS2 # endif #endif #if !defined WINDOWS_NATIVE # include # if HAVE_LANGINFO_CODESET # include # else # if 0 /* see comment below */ # include # endif # endif # ifdef __CYGWIN__ # define WIN32_LEAN_AND_MEAN # include # endif #elif defined WINDOWS_NATIVE # define WIN32_LEAN_AND_MEAN # include #endif #if defined OS2 # define INCL_DOS # include #endif /* For MB_CUR_MAX_L */ #if defined DARWIN7 # include #endif #if ENABLE_RELOCATABLE # include "relocatable.h" #else # define relocate(pathname) (pathname) # define relocate2(pathname,allocatedp) (*(allocatedp) = NULL, (pathname)) #endif /* Get LIBDIR. */ #ifndef LIBDIR # include "configmake.h" #endif /* Define O_NOFOLLOW to 0 on platforms where it does not exist. */ #ifndef O_NOFOLLOW # define O_NOFOLLOW 0 #endif #if defined _WIN32 || defined __WIN32__ || defined __CYGWIN__ || defined __EMX__ || defined __DJGPP__ /* Native Windows, Cygwin, OS/2, DOS */ # define ISSLASH(C) ((C) == '/' || (C) == '\\') #endif #ifndef DIRECTORY_SEPARATOR # define DIRECTORY_SEPARATOR '/' #endif #ifndef ISSLASH # define ISSLASH(C) ((C) == DIRECTORY_SEPARATOR) #endif #if HAVE_DECL_GETC_UNLOCKED # undef getc # define getc getc_unlocked #endif /* The following static variable is declared 'volatile' to avoid a possible multithread problem in the function get_charset_aliases. If we are running in a threaded environment, and if two threads initialize 'charset_aliases' simultaneously, both will produce the same value, and everything will be ok if the two assignments to 'charset_aliases' are atomic. But I don't know what will happen if the two assignments mix. */ #if __STDC__ != 1 # define volatile /* empty */ #endif /* Pointer to the contents of the charset.alias file, if it has already been read, else NULL. Its format is: ALIAS_1 '\0' CANONICAL_1 '\0' ... ALIAS_n '\0' CANONICAL_n '\0' '\0' */ static const char * volatile charset_aliases; /* Return a pointer to the contents of the charset.alias file. */ static const char * get_charset_aliases (void) { const char *cp; cp = charset_aliases; if (cp == NULL) { #if !(defined DARWIN7 || defined VMS || defined WINDOWS_NATIVE || defined __CYGWIN__ || defined OS2) char *malloc_dir = NULL; const char *dir; const char *base = "charset.alias"; char *file_name; /* Make it possible to override the charset.alias location. This is necessary for running the testsuite before "make install". */ dir = getenv ("CHARSETALIASDIR"); if (dir == NULL || dir[0] == '\0') dir = relocate2 (LIBDIR, &malloc_dir); /* Concatenate dir and base into freshly allocated file_name. */ { size_t dir_len = strlen (dir); size_t base_len = strlen (base); int add_slash = (dir_len > 0 && !ISSLASH (dir[dir_len - 1])); file_name = (char *) malloc (dir_len + add_slash + base_len + 1); if (file_name != NULL) { memcpy (file_name, dir, dir_len); if (add_slash) file_name[dir_len] = DIRECTORY_SEPARATOR; memcpy (file_name + dir_len + add_slash, base, base_len + 1); } } free (malloc_dir); if (file_name == NULL) /* Out of memory. Treat the file as empty. */ cp = ""; else { int fd; /* Open the file. Reject symbolic links on platforms that support O_NOFOLLOW. This is a security feature. Without it, an attacker could retrieve parts of the contents (namely, the tail of the first line that starts with "* ") of an arbitrary file by placing a symbolic link to that file under the name "charset.alias" in some writable directory and defining the environment variable CHARSETALIASDIR to point to that directory. */ fd = open (file_name, O_RDONLY | (HAVE_WORKING_O_NOFOLLOW ? O_NOFOLLOW : 0)); if (fd < 0) /* File not found. Treat it as empty. */ cp = ""; else { FILE *fp; fp = fdopen (fd, "r"); if (fp == NULL) { /* Out of memory. Treat the file as empty. */ close (fd); cp = ""; } else { /* Parse the file's contents. */ char *res_ptr = NULL; size_t res_size = 0; for (;;) { int c; char buf1[50+1]; char buf2[50+1]; size_t l1, l2; char *old_res_ptr; c = getc (fp); if (c == EOF) break; if (c == '\n' || c == ' ' || c == '\t') continue; if (c == '#') { /* Skip comment, to end of line. */ do c = getc (fp); while (!(c == EOF || c == '\n')); if (c == EOF) break; continue; } ungetc (c, fp); if (fscanf (fp, "%50s %50s", buf1, buf2) < 2) break; l1 = strlen (buf1); l2 = strlen (buf2); old_res_ptr = res_ptr; if (res_size == 0) { res_size = l1 + 1 + l2 + 1; res_ptr = (char *) malloc (res_size + 1); } else { res_size += l1 + 1 + l2 + 1; res_ptr = (char *) realloc (res_ptr, res_size + 1); } if (res_ptr == NULL) { /* Out of memory. */ res_size = 0; free (old_res_ptr); break; } strcpy (res_ptr + res_size - (l2 + 1) - (l1 + 1), buf1); strcpy (res_ptr + res_size - (l2 + 1), buf2); } fclose (fp); if (res_size == 0) cp = ""; else { *(res_ptr + res_size) = '\0'; cp = res_ptr; } } } free (file_name); } #else # if defined DARWIN7 /* To avoid the trouble of installing a file that is shared by many GNU packages -- many packaging systems have problems with this --, simply inline the aliases here. */ cp = "ISO8859-1" "\0" "ISO-8859-1" "\0" "ISO8859-2" "\0" "ISO-8859-2" "\0" "ISO8859-4" "\0" "ISO-8859-4" "\0" "ISO8859-5" "\0" "ISO-8859-5" "\0" "ISO8859-7" "\0" "ISO-8859-7" "\0" "ISO8859-9" "\0" "ISO-8859-9" "\0" "ISO8859-13" "\0" "ISO-8859-13" "\0" "ISO8859-15" "\0" "ISO-8859-15" "\0" "KOI8-R" "\0" "KOI8-R" "\0" "KOI8-U" "\0" "KOI8-U" "\0" "CP866" "\0" "CP866" "\0" "CP949" "\0" "CP949" "\0" "CP1131" "\0" "CP1131" "\0" "CP1251" "\0" "CP1251" "\0" "eucCN" "\0" "GB2312" "\0" "GB2312" "\0" "GB2312" "\0" "eucJP" "\0" "EUC-JP" "\0" "eucKR" "\0" "EUC-KR" "\0" "Big5" "\0" "BIG5" "\0" "Big5HKSCS" "\0" "BIG5-HKSCS" "\0" "GBK" "\0" "GBK" "\0" "GB18030" "\0" "GB18030" "\0" "SJIS" "\0" "SHIFT_JIS" "\0" "ARMSCII-8" "\0" "ARMSCII-8" "\0" "PT154" "\0" "PT154" "\0" /*"ISCII-DEV" "\0" "?" "\0"*/ "*" "\0" "UTF-8" "\0"; # endif # if defined VMS /* To avoid the troubles of an extra file charset.alias_vms in the sources of many GNU packages, simply inline the aliases here. */ /* The list of encodings is taken from the OpenVMS 7.3-1 documentation "Compaq C Run-Time Library Reference Manual for OpenVMS systems" section 10.7 "Handling Different Character Sets". */ cp = "ISO8859-1" "\0" "ISO-8859-1" "\0" "ISO8859-2" "\0" "ISO-8859-2" "\0" "ISO8859-5" "\0" "ISO-8859-5" "\0" "ISO8859-7" "\0" "ISO-8859-7" "\0" "ISO8859-8" "\0" "ISO-8859-8" "\0" "ISO8859-9" "\0" "ISO-8859-9" "\0" /* Japanese */ "eucJP" "\0" "EUC-JP" "\0" "SJIS" "\0" "SHIFT_JIS" "\0" "DECKANJI" "\0" "DEC-KANJI" "\0" "SDECKANJI" "\0" "EUC-JP" "\0" /* Chinese */ "eucTW" "\0" "EUC-TW" "\0" "DECHANYU" "\0" "DEC-HANYU" "\0" "DECHANZI" "\0" "GB2312" "\0" /* Korean */ "DECKOREAN" "\0" "EUC-KR" "\0"; # endif # if defined WINDOWS_NATIVE || defined __CYGWIN__ /* To avoid the troubles of installing a separate file in the same directory as the DLL and of retrieving the DLL's directory at runtime, simply inline the aliases here. */ cp = "CP936" "\0" "GBK" "\0" "CP1361" "\0" "JOHAB" "\0" "CP20127" "\0" "ASCII" "\0" "CP20866" "\0" "KOI8-R" "\0" "CP20936" "\0" "GB2312" "\0" "CP21866" "\0" "KOI8-RU" "\0" "CP28591" "\0" "ISO-8859-1" "\0" "CP28592" "\0" "ISO-8859-2" "\0" "CP28593" "\0" "ISO-8859-3" "\0" "CP28594" "\0" "ISO-8859-4" "\0" "CP28595" "\0" "ISO-8859-5" "\0" "CP28596" "\0" "ISO-8859-6" "\0" "CP28597" "\0" "ISO-8859-7" "\0" "CP28598" "\0" "ISO-8859-8" "\0" "CP28599" "\0" "ISO-8859-9" "\0" "CP28605" "\0" "ISO-8859-15" "\0" "CP38598" "\0" "ISO-8859-8" "\0" "CP51932" "\0" "EUC-JP" "\0" "CP51936" "\0" "GB2312" "\0" "CP51949" "\0" "EUC-KR" "\0" "CP51950" "\0" "EUC-TW" "\0" "CP54936" "\0" "GB18030" "\0" "CP65001" "\0" "UTF-8" "\0"; # endif # if defined OS2 /* To avoid the troubles of installing a separate file in the same directory as the DLL and of retrieving the DLL's directory at runtime, simply inline the aliases here. */ /* The list of encodings is taken from "List of OS/2 Codepages" by Alex Taylor: . See also "IBM Globalization - Code page identifiers": . */ cp = "CP813" "\0" "ISO-8859-7" "\0" "CP878" "\0" "KOI8-R" "\0" "CP819" "\0" "ISO-8859-1" "\0" "CP912" "\0" "ISO-8859-2" "\0" "CP913" "\0" "ISO-8859-3" "\0" "CP914" "\0" "ISO-8859-4" "\0" "CP915" "\0" "ISO-8859-5" "\0" "CP916" "\0" "ISO-8859-8" "\0" "CP920" "\0" "ISO-8859-9" "\0" "CP921" "\0" "ISO-8859-13" "\0" "CP923" "\0" "ISO-8859-15" "\0" "CP954" "\0" "EUC-JP" "\0" "CP964" "\0" "EUC-TW" "\0" "CP970" "\0" "EUC-KR" "\0" "CP1089" "\0" "ISO-8859-6" "\0" "CP1208" "\0" "UTF-8" "\0" "CP1381" "\0" "GB2312" "\0" "CP1386" "\0" "GBK" "\0" "CP3372" "\0" "EUC-JP" "\0"; # endif #endif charset_aliases = cp; } return cp; } /* Determine the current locale's character encoding, and canonicalize it into one of the canonical names listed in config.charset. The result must not be freed; it is statically allocated. If the canonical name cannot be determined, the result is a non-canonical name. */ #ifdef STATIC STATIC #endif const char * locale_charset (void) { const char *codeset; const char *aliases; #if !(defined WINDOWS_NATIVE || defined OS2) # if HAVE_LANGINFO_CODESET /* Most systems support nl_langinfo (CODESET) nowadays. */ codeset = nl_langinfo (CODESET); # ifdef __CYGWIN__ /* Cygwin < 1.7 does not have locales. nl_langinfo (CODESET) always returns "US-ASCII". Return the suffix of the locale name from the environment variables (if present) or the codepage as a number. */ if (codeset != NULL && strcmp (codeset, "US-ASCII") == 0) { const char *locale; static char buf[2 + 10 + 1]; locale = getenv ("LC_ALL"); if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_CTYPE"); if (locale == NULL || locale[0] == '\0') locale = getenv ("LANG"); } if (locale != NULL && locale[0] != '\0') { /* If the locale name contains an encoding after the dot, return it. */ const char *dot = strchr (locale, '.'); if (dot != NULL) { const char *modifier; dot++; /* Look for the possible @... trailer and remove it, if any. */ modifier = strchr (dot, '@'); if (modifier == NULL) return dot; if (modifier - dot < sizeof (buf)) { memcpy (buf, dot, modifier - dot); buf [modifier - dot] = '\0'; return buf; } } } /* The Windows API has a function returning the locale's codepage as a number: GetACP(). This encoding is used by Cygwin, unless the user has set the environment variable CYGWIN=codepage:oem (which very few people do). Output directed to console windows needs to be converted (to GetOEMCP() if the console is using a raster font, or to GetConsoleOutputCP() if it is using a TrueType font). Cygwin does this conversion transparently (see winsup/cygwin/fhandler_console.cc), converting to GetConsoleOutputCP(). This leads to correct results, except when SetConsoleOutputCP has been called and a raster font is in use. */ sprintf (buf, "CP%u", GetACP ()); codeset = buf; } # endif # else /* On old systems which lack it, use setlocale or getenv. */ const char *locale = NULL; /* But most old systems don't have a complete set of locales. Some (like SunOS 4 or DJGPP) have only the C locale. Therefore we don't use setlocale here; it would return "C" when it doesn't support the locale name the user has set. */ # if 0 locale = setlocale (LC_CTYPE, NULL); # endif if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_ALL"); if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_CTYPE"); if (locale == NULL || locale[0] == '\0') locale = getenv ("LANG"); } } /* On some old systems, one used to set locale = "iso8859_1". On others, you set it to "language_COUNTRY.charset". In any case, we resolve it through the charset.alias file. */ codeset = locale; # endif #elif defined WINDOWS_NATIVE static char buf[2 + 10 + 1]; /* The Windows API has a function returning the locale's codepage as a number, but the value doesn't change according to what the 'setlocale' call specified. So we use it as a last resort, in case the string returned by 'setlocale' doesn't specify the codepage. */ char *current_locale = setlocale (LC_ALL, NULL); char *pdot; /* If they set different locales for different categories, 'setlocale' will return a semi-colon separated list of locale values. To make sure we use the correct one, we choose LC_CTYPE. */ if (strchr (current_locale, ';')) current_locale = setlocale (LC_CTYPE, NULL); pdot = strrchr (current_locale, '.'); if (pdot && 2 + strlen (pdot + 1) + 1 <= sizeof (buf)) sprintf (buf, "CP%s", pdot + 1); else { /* The Windows API has a function returning the locale's codepage as a number: GetACP(). When the output goes to a console window, it needs to be provided in GetOEMCP() encoding if the console is using a raster font, or in GetConsoleOutputCP() encoding if it is using a TrueType font. But in GUI programs and for output sent to files and pipes, GetACP() encoding is the best bet. */ sprintf (buf, "CP%u", GetACP ()); } codeset = buf; #elif defined OS2 const char *locale; static char buf[2 + 10 + 1]; ULONG cp[3]; ULONG cplen; codeset = NULL; /* Allow user to override the codeset, as set in the operating system, with standard language environment variables. */ locale = getenv ("LC_ALL"); if (locale == NULL || locale[0] == '\0') { locale = getenv ("LC_CTYPE"); if (locale == NULL || locale[0] == '\0') locale = getenv ("LANG"); } if (locale != NULL && locale[0] != '\0') { /* If the locale name contains an encoding after the dot, return it. */ const char *dot = strchr (locale, '.'); if (dot != NULL) { const char *modifier; dot++; /* Look for the possible @... trailer and remove it, if any. */ modifier = strchr (dot, '@'); if (modifier == NULL) return dot; if (modifier - dot < sizeof (buf)) { memcpy (buf, dot, modifier - dot); buf [modifier - dot] = '\0'; return buf; } } /* For the POSIX locale, don't use the system's codepage. */ if (strcmp (locale, "C") == 0 || strcmp (locale, "POSIX") == 0) codeset = ""; } if (codeset == NULL) { /* OS/2 has a function returning the locale's codepage as a number. */ if (DosQueryCp (sizeof (cp), cp, &cplen)) codeset = ""; else { sprintf (buf, "CP%u", cp[0]); codeset = buf; } } #endif if (codeset == NULL) /* The canonical name cannot be determined. */ codeset = ""; /* Resolve alias. */ for (aliases = get_charset_aliases (); *aliases != '\0'; aliases += strlen (aliases) + 1, aliases += strlen (aliases) + 1) if (strcmp (codeset, aliases) == 0 || (aliases[0] == '*' && aliases[1] == '\0')) { codeset = aliases + strlen (aliases) + 1; break; } /* Don't return an empty string. GNU libc and GNU libiconv interpret the empty string as denoting "the locale's character encoding", thus GNU libiconv would call this function a second time. */ if (codeset[0] == '\0') codeset = "ASCII"; #ifdef DARWIN7 /* Mac OS X sets MB_CUR_MAX to 1 when LC_ALL=C, and "UTF-8" (the default codeset) does not work when MB_CUR_MAX is 1. */ if (strcmp (codeset, "UTF-8") == 0 && MB_CUR_MAX_L (uselocale (NULL)) <= 1) codeset = "ASCII"; #endif return codeset; } gnuastro-0.5/bootstrapped/lib/localcharset.h0000644000175000017500000000243313217200021016220 00000000000000/* Determine a canonical name for the current locale's character encoding. Copyright (C) 2000-2003, 2009-2017 Free Software Foundation, Inc. This file is part of the GNU CHARSET Library. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _LOCALCHARSET_H #define _LOCALCHARSET_H #ifdef __cplusplus extern "C" { #endif /* Determine the current locale's character encoding, and canonicalize it into one of the canonical names listed in config.charset. The result must not be freed; it is statically allocated. If the canonical name cannot be determined, the result is a non-canonical name. */ extern const char * locale_charset (void); #ifdef __cplusplus } #endif #endif /* _LOCALCHARSET_H */ gnuastro-0.5/bootstrapped/lib/hard-locale.c0000644000175000017500000000414613217200021015725 00000000000000/* hard-locale.c -- Determine whether a locale is hard. Copyright (C) 1997-1999, 2002-2004, 2006-2007, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "hard-locale.h" #include #include #include #ifdef __GLIBC__ # define GLIBC_VERSION __GLIBC__ #elif defined __UCLIBC__ # define GLIBC_VERSION 2 #else # define GLIBC_VERSION 0 #endif /* Return true if the current CATEGORY locale is hard, i.e. if you can't get away with assuming traditional C or POSIX behavior. */ bool hard_locale (int category) { bool hard = true; char const *p = setlocale (category, NULL); if (p) { if (2 <= GLIBC_VERSION) { if (strcmp (p, "C") == 0 || strcmp (p, "POSIX") == 0) hard = false; } else { char *locale = strdup (p); if (locale) { /* Temporarily set the locale to the "C" and "POSIX" locales to find their names, so that we can determine whether one or the other is the caller's locale. */ if (((p = setlocale (category, "C")) && strcmp (p, locale) == 0) || ((p = setlocale (category, "POSIX")) && strcmp (p, locale) == 0)) hard = false; /* Restore the caller's locale. */ setlocale (category, locale); free (locale); } } } return hard; } gnuastro-0.5/bootstrapped/lib/gettext.h0000644000175000017500000002410013217200021015233 00000000000000/* Convenience header for conditional use of GNU . Copyright (C) 1995-1998, 2000-2002, 2004-2006, 2009-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef _LIBGETTEXT_H #define _LIBGETTEXT_H 1 /* NLS can be disabled through the configure --disable-nls option or through "#define ENABLE NLS 0" before including this file. */ #if defined ENABLE_NLS && ENABLE_NLS /* Get declarations of GNU message catalog functions. */ # include /* You can set the DEFAULT_TEXT_DOMAIN macro to specify the domain used by the gettext() and ngettext() macros. This is an alternative to calling textdomain(), and is useful for libraries. */ # ifdef DEFAULT_TEXT_DOMAIN # undef gettext # define gettext(Msgid) \ dgettext (DEFAULT_TEXT_DOMAIN, Msgid) # undef ngettext # define ngettext(Msgid1, Msgid2, N) \ dngettext (DEFAULT_TEXT_DOMAIN, Msgid1, Msgid2, N) # endif #else /* Solaris /usr/include/locale.h includes /usr/include/libintl.h, which chokes if dcgettext is defined as a macro. So include it now, to make later inclusions of a NOP. We don't include as well because people using "gettext.h" will not include , and also including would fail on SunOS 4, whereas is OK. */ #if defined(__sun) # include #endif /* Many header files from the libstdc++ coming with g++ 3.3 or newer include , which chokes if dcgettext is defined as a macro. So include it now, to make later inclusions of a NOP. */ #if defined(__cplusplus) && defined(__GNUG__) && (__GNUC__ >= 3) # include # if (__GLIBC__ >= 2 && !defined __UCLIBC__) || _GLIBCXX_HAVE_LIBINTL_H # include # endif #endif /* Disabled NLS. The casts to 'const char *' serve the purpose of producing warnings for invalid uses of the value returned from these functions. On pre-ANSI systems without 'const', the config.h file is supposed to contain "#define const". */ # undef gettext # define gettext(Msgid) ((const char *) (Msgid)) # undef dgettext # define dgettext(Domainname, Msgid) ((void) (Domainname), gettext (Msgid)) # undef dcgettext # define dcgettext(Domainname, Msgid, Category) \ ((void) (Category), dgettext (Domainname, Msgid)) # undef ngettext # define ngettext(Msgid1, Msgid2, N) \ ((N) == 1 \ ? ((void) (Msgid2), (const char *) (Msgid1)) \ : ((void) (Msgid1), (const char *) (Msgid2))) # undef dngettext # define dngettext(Domainname, Msgid1, Msgid2, N) \ ((void) (Domainname), ngettext (Msgid1, Msgid2, N)) # undef dcngettext # define dcngettext(Domainname, Msgid1, Msgid2, N, Category) \ ((void) (Category), dngettext (Domainname, Msgid1, Msgid2, N)) # undef textdomain # define textdomain(Domainname) ((const char *) (Domainname)) # undef bindtextdomain # define bindtextdomain(Domainname, Dirname) \ ((void) (Domainname), (const char *) (Dirname)) # undef bind_textdomain_codeset # define bind_textdomain_codeset(Domainname, Codeset) \ ((void) (Domainname), (const char *) (Codeset)) #endif /* Prefer gnulib's setlocale override over libintl's setlocale override. */ #ifdef GNULIB_defined_setlocale # undef setlocale # define setlocale rpl_setlocale #endif /* A pseudo function call that serves as a marker for the automated extraction of messages, but does not call gettext(). The run-time translation is done at a different place in the code. The argument, String, should be a literal string. Concatenated strings and other string expressions won't work. The macro's expansion is not parenthesized, so that it is suitable as initializer for static 'char[]' or 'const char[]' variables. */ #define gettext_noop(String) String /* The separator between msgctxt and msgid in a .mo file. */ #define GETTEXT_CONTEXT_GLUE "\004" /* Pseudo function calls, taking a MSGCTXT and a MSGID instead of just a MSGID. MSGCTXT and MSGID must be string literals. MSGCTXT should be short and rarely need to change. The letter 'p' stands for 'particular' or 'special'. */ #ifdef DEFAULT_TEXT_DOMAIN # define pgettext(Msgctxt, Msgid) \ pgettext_aux (DEFAULT_TEXT_DOMAIN, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, LC_MESSAGES) #else # define pgettext(Msgctxt, Msgid) \ pgettext_aux (NULL, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, LC_MESSAGES) #endif #define dpgettext(Domainname, Msgctxt, Msgid) \ pgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, LC_MESSAGES) #define dcpgettext(Domainname, Msgctxt, Msgid, Category) \ pgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, Category) #ifdef DEFAULT_TEXT_DOMAIN # define npgettext(Msgctxt, Msgid, MsgidPlural, N) \ npgettext_aux (DEFAULT_TEXT_DOMAIN, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, LC_MESSAGES) #else # define npgettext(Msgctxt, Msgid, MsgidPlural, N) \ npgettext_aux (NULL, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, LC_MESSAGES) #endif #define dnpgettext(Domainname, Msgctxt, Msgid, MsgidPlural, N) \ npgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, LC_MESSAGES) #define dcnpgettext(Domainname, Msgctxt, Msgid, MsgidPlural, N, Category) \ npgettext_aux (Domainname, Msgctxt GETTEXT_CONTEXT_GLUE Msgid, Msgid, MsgidPlural, N, Category) #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * pgettext_aux (const char *domain, const char *msg_ctxt_id, const char *msgid, int category) { const char *translation = dcgettext (domain, msg_ctxt_id, category); if (translation == msg_ctxt_id) return msgid; else return translation; } #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * npgettext_aux (const char *domain, const char *msg_ctxt_id, const char *msgid, const char *msgid_plural, unsigned long int n, int category) { const char *translation = dcngettext (domain, msg_ctxt_id, msgid_plural, n, category); if (translation == msg_ctxt_id || translation == msgid_plural) return (n == 1 ? msgid : msgid_plural); else return translation; } /* The same thing extended for non-constant arguments. Here MSGCTXT and MSGID can be arbitrary expressions. But for string literals these macros are less efficient than those above. */ #include #if (((__GNUC__ >= 3 || __GNUG__ >= 2) && !defined __STRICT_ANSI__) \ /* || __STDC_VERSION__ == 199901L || (__STDC_VERSION__ >= 201112L && !defined __STDC_NO_VLA__) */ ) # define _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS 1 #else # define _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS 0 #endif #if !_LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS #include #endif #define pgettext_expr(Msgctxt, Msgid) \ dcpgettext_expr (NULL, Msgctxt, Msgid, LC_MESSAGES) #define dpgettext_expr(Domainname, Msgctxt, Msgid) \ dcpgettext_expr (Domainname, Msgctxt, Msgid, LC_MESSAGES) #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * dcpgettext_expr (const char *domain, const char *msgctxt, const char *msgid, int category) { size_t msgctxt_len = strlen (msgctxt) + 1; size_t msgid_len = strlen (msgid) + 1; const char *translation; #if _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS char msg_ctxt_id[msgctxt_len + msgid_len]; #else char buf[1024]; char *msg_ctxt_id = (msgctxt_len + msgid_len <= sizeof (buf) ? buf : (char *) malloc (msgctxt_len + msgid_len)); if (msg_ctxt_id != NULL) #endif { int found_translation; memcpy (msg_ctxt_id, msgctxt, msgctxt_len - 1); msg_ctxt_id[msgctxt_len - 1] = '\004'; memcpy (msg_ctxt_id + msgctxt_len, msgid, msgid_len); translation = dcgettext (domain, msg_ctxt_id, category); found_translation = (translation != msg_ctxt_id); #if !_LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS if (msg_ctxt_id != buf) free (msg_ctxt_id); #endif if (found_translation) return translation; } return msgid; } #define npgettext_expr(Msgctxt, Msgid, MsgidPlural, N) \ dcnpgettext_expr (NULL, Msgctxt, Msgid, MsgidPlural, N, LC_MESSAGES) #define dnpgettext_expr(Domainname, Msgctxt, Msgid, MsgidPlural, N) \ dcnpgettext_expr (Domainname, Msgctxt, Msgid, MsgidPlural, N, LC_MESSAGES) #ifdef __GNUC__ __inline #else #ifdef __cplusplus inline #endif #endif static const char * dcnpgettext_expr (const char *domain, const char *msgctxt, const char *msgid, const char *msgid_plural, unsigned long int n, int category) { size_t msgctxt_len = strlen (msgctxt) + 1; size_t msgid_len = strlen (msgid) + 1; const char *translation; #if _LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS char msg_ctxt_id[msgctxt_len + msgid_len]; #else char buf[1024]; char *msg_ctxt_id = (msgctxt_len + msgid_len <= sizeof (buf) ? buf : (char *) malloc (msgctxt_len + msgid_len)); if (msg_ctxt_id != NULL) #endif { int found_translation; memcpy (msg_ctxt_id, msgctxt, msgctxt_len - 1); msg_ctxt_id[msgctxt_len - 1] = '\004'; memcpy (msg_ctxt_id + msgctxt_len, msgid, msgid_len); translation = dcngettext (domain, msg_ctxt_id, msgid_plural, n, category); found_translation = !(translation == msg_ctxt_id || translation == msgid_plural); #if !_LIBGETTEXT_HAVE_VARIABLE_SIZE_ARRAYS if (msg_ctxt_id != buf) free (msg_ctxt_id); #endif if (found_translation) return translation; } return (n == 1 ? msgid : msgid_plural); } #endif /* _LIBGETTEXT_H */ gnuastro-0.5/bootstrapped/lib/getprogname.c0000644000175000017500000001335113217200021016060 00000000000000/* Program name management. Copyright (C) 2016-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include "getprogname.h" #include /* get program_invocation_name declaration */ #include /* get __argv declaration */ #ifdef _AIX # include # include # include #endif #ifdef __MVS__ # ifndef _OPEN_SYS # define _OPEN_SYS # endif # include # include #endif #ifdef __hpux # include # include # include # include #endif #ifdef __sgi # include # include # include # include # include #endif #include "dirname.h" #ifndef HAVE_GETPROGNAME /* not Mac OS X, FreeBSD, NetBSD, OpenBSD >= 5.4, Cygwin */ char const * getprogname (void) { # if HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME /* glibc, BeOS */ /* https://www.gnu.org/software/libc/manual/html_node/Error-Messages.html */ return program_invocation_short_name; # elif HAVE_DECL_PROGRAM_INVOCATION_NAME /* glibc, BeOS */ /* https://www.gnu.org/software/libc/manual/html_node/Error-Messages.html */ return last_component (program_invocation_name); # elif HAVE_GETEXECNAME /* Solaris */ /* https://docs.oracle.com/cd/E19253-01/816-5168/6mbb3hrb1/index.html */ const char *p = getexecname (); if (!p) p = "?"; return last_component (p); # elif HAVE_DECL___ARGV /* mingw, MSVC */ /* https://msdn.microsoft.com/en-us/library/dn727674.aspx */ const char *p = __argv && __argv[0] ? __argv[0] : "?"; return last_component (p); # elif HAVE_VAR___PROGNAME /* OpenBSD, QNX */ /* https://man.openbsd.org/style.9 */ /* http://www.qnx.de/developers/docs/6.5.0/index.jsp?topic=%2Fcom.qnx.doc.neutrino_lib_ref%2Fp%2F__progname.html */ /* Be careful to declare this only when we absolutely need it (OpenBSD 5.1), rather than when it's available. Otherwise, its mere declaration makes program_invocation_short_name malfunction (have zero length) with Fedora 25's glibc. */ extern char *__progname; const char *p = __progname; return p && p[0] ? p : "?"; # elif _AIX /* AIX */ /* Idea by Bastien ROUCARIÈS, https://lists.gnu.org/r/bug-gnulib/2010-12/msg00095.html Reference: https://www.ibm.com/support/knowledgecenter/en/ssw_aix_61/com.ibm.aix.basetrf1/getprocs.htm */ static char *p; static int first = 1; if (first) { first = 0; pid_t pid = getpid (); struct procentry64 procs; p = (0 < getprocs64 (&procs, sizeof procs, NULL, 0, &pid, 1) ? strdup (procs.pi_comm) : NULL); if (!p) p = "?"; } return p; # elif defined __hpux static char *p; static int first = 1; if (first) { first = 0; pid_t pid = getpid (); struct pst_status status; p = (0 < pstat_getproc (&status, sizeof status, 0, pid) ? strdup (status.pst_ucomm) : NULL); if (!p) p = "?"; } return p; # elif __MVS__ /* z/OS */ /* https://www.ibm.com/support/knowledgecenter/SSLTBW_2.1.0/com.ibm.zos.v2r1.bpxbd00/rtwgetp.htm */ static char *p = "?"; static int first = 1; if (first) { pid_t pid = getpid (); int token; W_PSPROC buf; first = 0; memset (&buf, 0, sizeof(buf)); buf.ps_cmdptr = (char *) malloc (buf.ps_cmdlen = PS_CMDBLEN_LONG); buf.ps_conttyptr = (char *) malloc (buf.ps_conttylen = PS_CONTTYBLEN); buf.ps_pathptr = (char *) malloc (buf.ps_pathlen = PS_PATHBLEN); if (buf.ps_cmdptr && buf.ps_conttyptr && buf.ps_pathptr) { for (token = 0; token >= 0; token = w_getpsent (token, &buf, sizeof(buf))) { if (token > 0 && buf.ps_pid == pid) { char *s = strdup (last_component (buf.ps_pathptr)); if (s) p = s; break; } } } free (buf.ps_cmdptr); free (buf.ps_conttyptr); free (buf.ps_pathptr); } return p; # elif defined __sgi /* IRIX */ char filename[50]; int fd; sprintf (filename, "/proc/pinfo/%d", (int) getpid ()); fd = open (filename, O_RDONLY); if (0 <= fd) { prpsinfo_t buf; int ioctl_ok = 0 <= ioctl (fd, PIOCPSINFO, &buf); close (fd); if (ioctl_ok) { char *name = buf.pr_fname; size_t namesize = sizeof buf.pr_fname; char *namenul = memchr (name, '\0', namesize); size_t namelen = namenul ? namenul - name : namesize; char *namecopy = malloc (namelen + 1); if (namecopy) { namecopy[namelen] = 0; return memcpy (namecopy, name, namelen); } } } return NULL; # else # error "getprogname module not ported to this OS" # endif } #endif gnuastro-0.5/bootstrapped/lib/getprogname.h0000644000175000017500000000217413217200021016066 00000000000000/* Program name management. Copyright (C) 2016-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GL_GETPROGNAME_H #define _GL_GETPROGNAME_H #include #ifdef __cplusplus extern "C" { #endif /* Return the base name of the executing program. On native Windows this will usually end in ".exe" or ".EXE". */ #ifndef HAVE_GETPROGNAME extern char const *getprogname (void) # ifdef HAVE_DECL_PROGRAM_INVOCATION_NAME _GL_ATTRIBUTE_PURE # endif ; #endif #ifdef __cplusplus } #endif #endif gnuastro-0.5/bootstrapped/lib/stripslash.c0000644000175000017500000000304213217200021015740 00000000000000/* stripslash.c -- remove redundant trailing slashes from a file name Copyright (C) 1990, 2001, 2003-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "dirname.h" /* Remove trailing slashes from FILE. Return true if a trailing slash was removed. This is useful when using file name completion from a shell that adds a "/" after directory names (such as tcsh and bash), because on symlinks to directories, several system calls have different semantics according to whether a trailing slash is present. */ bool strip_trailing_slashes (char *file) { char *base = last_component (file); char *base_lim; bool had_slash; /* last_component returns "" for file system roots, but we need to turn "///" into "/". */ if (! *base) base = file; base_lim = base + base_len (base); had_slash = (*base_lim != '\0'); *base_lim = '\0'; return had_slash; } gnuastro-0.5/bootstrapped/lib/basename-lgpl.c0000644000175000017500000000406213217200020016255 00000000000000/* basename.c -- return the last element in a file name Copyright (C) 1990, 1998-2001, 2003-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "dirname.h" #include /* Return the address of the last file name component of NAME. If NAME has no relative file name components because it is a file system root, return the empty string. */ char * last_component (char const *name) { char const *base = name + FILE_SYSTEM_PREFIX_LEN (name); char const *p; bool saw_slash = false; while (ISSLASH (*base)) base++; for (p = base; *p; p++) { if (ISSLASH (*p)) saw_slash = true; else if (saw_slash) { base = p; saw_slash = false; } } return (char *) base; } /* Return the length of the basename NAME. Typically NAME is the value returned by base_name or last_component. Act like strlen (NAME), except omit all trailing slashes. */ size_t base_len (char const *name) { size_t len; size_t prefix_len = FILE_SYSTEM_PREFIX_LEN (name); for (len = strlen (name); 1 < len && ISSLASH (name[len - 1]); len--) continue; if (DOUBLE_SLASH_IS_DISTINCT_ROOT && len == 1 && ISSLASH (name[0]) && ISSLASH (name[1]) && ! name[2]) return 2; if (FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE && prefix_len && len == prefix_len && ISSLASH (name[prefix_len])) return prefix_len + 1; return len; } gnuastro-0.5/bootstrapped/lib/dirname-lgpl.c0000644000175000017500000000612113217200021016120 00000000000000/* dirname.c -- return all but the last element in a file name Copyright (C) 1990, 1998, 2000-2001, 2003-2006, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include #include "dirname.h" #include #include /* Return the length of the prefix of FILE that will be used by dir_name. If FILE is in the working directory, this returns zero even though 'dir_name (FILE)' will return ".". Works properly even if there are trailing slashes (by effectively ignoring them). */ size_t dir_len (char const *file) { size_t prefix_length = FILE_SYSTEM_PREFIX_LEN (file); size_t length; /* Advance prefix_length beyond important leading slashes. */ prefix_length += (prefix_length != 0 ? (FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE && ISSLASH (file[prefix_length])) : (ISSLASH (file[0]) ? ((DOUBLE_SLASH_IS_DISTINCT_ROOT && ISSLASH (file[1]) && ! ISSLASH (file[2]) ? 2 : 1)) : 0)); /* Strip the basename and any redundant slashes before it. */ for (length = last_component (file) - file; prefix_length < length; length--) if (! ISSLASH (file[length - 1])) break; return length; } /* In general, we can't use the builtin 'dirname' function if available, since it has different meanings in different environments. In some environments the builtin 'dirname' modifies its argument. Return the leading directories part of FILE, allocated with malloc. Works properly even if there are trailing slashes (by effectively ignoring them). Return NULL on failure. If lstat (FILE) would succeed, then { chdir (dir_name (FILE)); lstat (base_name (FILE)); } will access the same file. Likewise, if the sequence { chdir (dir_name (FILE)); rename (base_name (FILE), "foo"); } succeeds, you have renamed FILE to "foo" in the same directory FILE was in. */ char * mdir_name (char const *file) { size_t length = dir_len (file); bool append_dot = (length == 0 || (FILE_SYSTEM_DRIVE_PREFIX_CAN_BE_RELATIVE && length == FILE_SYSTEM_PREFIX_LEN (file) && file[2] != '\0' && ! ISSLASH (file[2]))); char *dir = malloc (length + append_dot + 1); if (!dir) return NULL; memcpy (dir, file, length); if (append_dot) dir[length++] = '.'; dir[length] = '\0'; return dir; } gnuastro-0.5/bootstrapped/lib/c-ctype.c0000644000175000017500000000012213217200020015103 00000000000000#include #define C_CTYPE_INLINE _GL_EXTERN_INLINE #include "c-ctype.h" gnuastro-0.5/bootstrapped/lib/c-ctype.h0000644000175000017500000002240713217200021015123 00000000000000/* Character handling in C locale. These functions work like the corresponding functions in , except that they have the C (POSIX) locale hardwired, whereas the functions' behaviour depends on the current locale set via setlocale. Copyright (C) 2000-2003, 2006, 2008-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ #ifndef C_CTYPE_H #define C_CTYPE_H #include #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef C_CTYPE_INLINE # define C_CTYPE_INLINE _GL_INLINE #endif #ifdef __cplusplus extern "C" { #endif /* The functions defined in this file assume the "C" locale and a character set without diacritics (ASCII-US or EBCDIC-US or something like that). Even if the "C" locale on a particular system is an extension of the ASCII character set (like on BeOS, where it is UTF-8, or on AmigaOS, where it is ISO-8859-1), the functions in this file recognize only the ASCII characters. */ #if (' ' == 32) && ('!' == 33) && ('"' == 34) && ('#' == 35) \ && ('%' == 37) && ('&' == 38) && ('\'' == 39) && ('(' == 40) \ && (')' == 41) && ('*' == 42) && ('+' == 43) && (',' == 44) \ && ('-' == 45) && ('.' == 46) && ('/' == 47) && ('0' == 48) \ && ('1' == 49) && ('2' == 50) && ('3' == 51) && ('4' == 52) \ && ('5' == 53) && ('6' == 54) && ('7' == 55) && ('8' == 56) \ && ('9' == 57) && (':' == 58) && (';' == 59) && ('<' == 60) \ && ('=' == 61) && ('>' == 62) && ('?' == 63) && ('A' == 65) \ && ('B' == 66) && ('C' == 67) && ('D' == 68) && ('E' == 69) \ && ('F' == 70) && ('G' == 71) && ('H' == 72) && ('I' == 73) \ && ('J' == 74) && ('K' == 75) && ('L' == 76) && ('M' == 77) \ && ('N' == 78) && ('O' == 79) && ('P' == 80) && ('Q' == 81) \ && ('R' == 82) && ('S' == 83) && ('T' == 84) && ('U' == 85) \ && ('V' == 86) && ('W' == 87) && ('X' == 88) && ('Y' == 89) \ && ('Z' == 90) && ('[' == 91) && ('\\' == 92) && (']' == 93) \ && ('^' == 94) && ('_' == 95) && ('a' == 97) && ('b' == 98) \ && ('c' == 99) && ('d' == 100) && ('e' == 101) && ('f' == 102) \ && ('g' == 103) && ('h' == 104) && ('i' == 105) && ('j' == 106) \ && ('k' == 107) && ('l' == 108) && ('m' == 109) && ('n' == 110) \ && ('o' == 111) && ('p' == 112) && ('q' == 113) && ('r' == 114) \ && ('s' == 115) && ('t' == 116) && ('u' == 117) && ('v' == 118) \ && ('w' == 119) && ('x' == 120) && ('y' == 121) && ('z' == 122) \ && ('{' == 123) && ('|' == 124) && ('}' == 125) && ('~' == 126) /* The character set is ASCII or one of its variants or extensions, not EBCDIC. Testing the value of '\n' and '\r' is not relevant. */ # define C_CTYPE_ASCII 1 #elif ! (' ' == '\x40' && '0' == '\xf0' \ && 'A' == '\xc1' && 'J' == '\xd1' && 'S' == '\xe2' \ && 'a' == '\x81' && 'j' == '\x91' && 's' == '\xa2') # error "Only ASCII and EBCDIC are supported" #endif #if 'A' < 0 # error "EBCDIC and char is signed -- not supported" #endif /* Cases for control characters. */ #define _C_CTYPE_CNTRL \ case '\a': case '\b': case '\f': case '\n': \ case '\r': case '\t': case '\v': \ _C_CTYPE_OTHER_CNTRL /* ASCII control characters other than those with \-letter escapes. */ #if C_CTYPE_ASCII # define _C_CTYPE_OTHER_CNTRL \ case '\x00': case '\x01': case '\x02': case '\x03': \ case '\x04': case '\x05': case '\x06': case '\x0e': \ case '\x0f': case '\x10': case '\x11': case '\x12': \ case '\x13': case '\x14': case '\x15': case '\x16': \ case '\x17': case '\x18': case '\x19': case '\x1a': \ case '\x1b': case '\x1c': case '\x1d': case '\x1e': \ case '\x1f': case '\x7f' #else /* Use EBCDIC code page 1047's assignments for ASCII control chars; assume all EBCDIC code pages agree about these assignments. */ # define _C_CTYPE_OTHER_CNTRL \ case '\x00': case '\x01': case '\x02': case '\x03': \ case '\x07': case '\x0e': case '\x0f': case '\x10': \ case '\x11': case '\x12': case '\x13': case '\x18': \ case '\x19': case '\x1c': case '\x1d': case '\x1e': \ case '\x1f': case '\x26': case '\x27': case '\x2d': \ case '\x2e': case '\x32': case '\x37': case '\x3c': \ case '\x3d': case '\x3f' #endif /* Cases for lowercase hex letters, and lowercase letters, all offset by N. */ #define _C_CTYPE_LOWER_A_THRU_F_N(N) \ case 'a' + (N): case 'b' + (N): case 'c' + (N): case 'd' + (N): \ case 'e' + (N): case 'f' + (N) #define _C_CTYPE_LOWER_N(N) \ _C_CTYPE_LOWER_A_THRU_F_N(N): \ case 'g' + (N): case 'h' + (N): case 'i' + (N): case 'j' + (N): \ case 'k' + (N): case 'l' + (N): case 'm' + (N): case 'n' + (N): \ case 'o' + (N): case 'p' + (N): case 'q' + (N): case 'r' + (N): \ case 's' + (N): case 't' + (N): case 'u' + (N): case 'v' + (N): \ case 'w' + (N): case 'x' + (N): case 'y' + (N): case 'z' + (N) /* Cases for hex letters, digits, lower, punct, and upper. */ #define _C_CTYPE_A_THRU_F \ _C_CTYPE_LOWER_A_THRU_F_N (0): \ _C_CTYPE_LOWER_A_THRU_F_N ('A' - 'a') #define _C_CTYPE_DIGIT \ case '0': case '1': case '2': case '3': \ case '4': case '5': case '6': case '7': \ case '8': case '9' #define _C_CTYPE_LOWER _C_CTYPE_LOWER_N (0) #define _C_CTYPE_PUNCT \ case '!': case '"': case '#': case '$': \ case '%': case '&': case '\'': case '(': \ case ')': case '*': case '+': case ',': \ case '-': case '.': case '/': case ':': \ case ';': case '<': case '=': case '>': \ case '?': case '@': case '[': case '\\': \ case ']': case '^': case '_': case '`': \ case '{': case '|': case '}': case '~' #define _C_CTYPE_UPPER _C_CTYPE_LOWER_N ('A' - 'a') /* Function definitions. */ /* Unlike the functions in , which require an argument in the range of the 'unsigned char' type, the functions here operate on values that are in the 'unsigned char' range or in the 'char' range. In other words, when you have a 'char' value, you need to cast it before using it as argument to a function: const char *s = ...; if (isalpha ((unsigned char) *s)) ... but you don't need to cast it for the functions defined in this file: const char *s = ...; if (c_isalpha (*s)) ... */ C_CTYPE_INLINE bool c_isalnum (int c) { switch (c) { _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_isalpha (int c) { switch (c) { _C_CTYPE_LOWER: _C_CTYPE_UPPER: return true; default: return false; } } /* The function isascii is not locale dependent. Its use in EBCDIC is questionable. */ C_CTYPE_INLINE bool c_isascii (int c) { switch (c) { case ' ': _C_CTYPE_CNTRL: _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_PUNCT: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_isblank (int c) { return c == ' ' || c == '\t'; } C_CTYPE_INLINE bool c_iscntrl (int c) { switch (c) { _C_CTYPE_CNTRL: return true; default: return false; } } C_CTYPE_INLINE bool c_isdigit (int c) { switch (c) { _C_CTYPE_DIGIT: return true; default: return false; } } C_CTYPE_INLINE bool c_isgraph (int c) { switch (c) { _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_PUNCT: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_islower (int c) { switch (c) { _C_CTYPE_LOWER: return true; default: return false; } } C_CTYPE_INLINE bool c_isprint (int c) { switch (c) { case ' ': _C_CTYPE_DIGIT: _C_CTYPE_LOWER: _C_CTYPE_PUNCT: _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_ispunct (int c) { switch (c) { _C_CTYPE_PUNCT: return true; default: return false; } } C_CTYPE_INLINE bool c_isspace (int c) { switch (c) { case ' ': case '\t': case '\n': case '\v': case '\f': case '\r': return true; default: return false; } } C_CTYPE_INLINE bool c_isupper (int c) { switch (c) { _C_CTYPE_UPPER: return true; default: return false; } } C_CTYPE_INLINE bool c_isxdigit (int c) { switch (c) { _C_CTYPE_DIGIT: _C_CTYPE_A_THRU_F: return true; default: return false; } } C_CTYPE_INLINE int c_tolower (int c) { switch (c) { _C_CTYPE_UPPER: return c - 'A' + 'a'; default: return c; } } C_CTYPE_INLINE int c_toupper (int c) { switch (c) { _C_CTYPE_LOWER: return c - 'a' + 'A'; default: return c; } } #ifdef __cplusplus } #endif _GL_INLINE_HEADER_END #endif /* C_CTYPE_H */ gnuastro-0.5/bootstrapped/lib/argp-xinl.c0000644000175000017500000000256613217200020015456 00000000000000/* Real definitions for extern inline functions in argp.h Copyright (C) 1997-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #if defined _LIBC || defined HAVE_FEATURES_H # include #endif #ifndef __USE_EXTERN_INLINES # define __USE_EXTERN_INLINES 1 #endif #ifdef _LIBC # define ARGP_EI #else # define ARGP_EI _GL_EXTERN_INLINE #endif #undef __OPTIMIZE__ #define __OPTIMIZE__ 1 #include "argp.h" /* Add weak aliases. */ #if _LIBC - 0 && defined (weak_alias) weak_alias (__argp_usage, argp_usage) weak_alias (__option_is_short, _option_is_short) weak_alias (__option_is_end, _option_is_end) #endif gnuastro-0.5/bootstrapped/lib/argp-pvh.c0000644000175000017500000000253613217200020015276 00000000000000/* Default definition for ARGP_PROGRAM_VERSION_HOOK. Copyright (C) 1996-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include "argp.h" /* If set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which calls this function with a stream to print the version to and a pointer to the current parsing state, and then exits (unless the ARGP_NO_EXIT flag is used). This variable takes precedent over ARGP_PROGRAM_VERSION. */ void (*argp_program_version_hook) (FILE *stream, struct argp_state *state) = NULL; gnuastro-0.5/bootstrapped/lib/argp-pv.c0000644000175000017500000000301613217200020015120 00000000000000/* Default definition for ARGP_PROGRAM_VERSION. Copyright (C) 1996-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* If set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which will print this string followed by a newline and exit (unless the ARGP_NO_EXIT flag is used). Overridden by ARGP_PROGRAM_VERSION_HOOK. */ const char *argp_program_version /* This variable should be zero-initialized. On most systems, putting it into BSS is sufficient. Not so on Mac OS X 10.3 and 10.4, see . */ #if defined __ELF__ /* On ELF systems, variables in BSS behave well. */ #else = (const char *) 0 #endif ; gnuastro-0.5/bootstrapped/lib/argp-pin.c0000644000175000017500000000226213217200020015263 00000000000000/* Full and short program names for argp module Copyright (C) 2005, 2009-2017 Free Software Foundation, Inc. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #ifndef HAVE_PROGRAM_INVOCATION_SHORT_NAME char *program_invocation_short_name = 0; #endif #ifndef HAVE_PROGRAM_INVOCATION_NAME char *program_invocation_name = 0; #endif #if (defined HAVE_PROGRAM_INVOCATION_SHORT_NAME \ && defined HAVE_PROGRAM_INVOCATION_NAME) /* This declaration is solely to ensure that after preprocessing this file is never empty. */ typedef int dummy; #endif gnuastro-0.5/bootstrapped/lib/argp-parse.c0000644000175000017500000007577313217200020015630 00000000000000/* Hierarchical argument parsing, layered over getopt Copyright (C) 1995-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include #include #include #include #ifdef _LIBC # include # undef dgettext # define dgettext(domain, msgid) \ __dcgettext (domain, msgid, LC_MESSAGES) #else # include "gettext.h" #endif #define N_(msgid) msgid #include "argp.h" #include "argp-namefrob.h" #define alignto(n, d) ((((n) + (d) - 1) / (d)) * (d)) /* Getopt return values. */ #define KEY_END (-1) /* The end of the options. */ #define KEY_ARG 1 /* A non-option argument. */ #define KEY_ERR '?' /* An error parsing the options. */ /* The meta-argument used to prevent any further arguments being interpreted as options. */ #define QUOTE "--" /* The number of bits we steal in a long-option value for our own use. */ #define GROUP_BITS CHAR_BIT /* The number of bits available for the user value. */ #define USER_BITS ((sizeof ((struct option *)0)->val * CHAR_BIT) - GROUP_BITS) #define USER_MASK ((1 << USER_BITS) - 1) /* EZ alias for ARGP_ERR_UNKNOWN. */ #define EBADKEY ARGP_ERR_UNKNOWN /* Default options. */ /* When argp is given the --HANG switch, _ARGP_HANG is set and argp will sleep for one second intervals, decrementing _ARGP_HANG until it's zero. Thus you can force the program to continue by attaching a debugger and setting it to 0 yourself. */ static volatile int _argp_hang; #define OPT_PROGNAME -2 #define OPT_USAGE -3 #define OPT_HANG -4 static const struct argp_option argp_default_options[] = { {"help", '?', 0, 0, N_("give this help list"), -1}, {"usage", OPT_USAGE, 0, 0, N_("give a short usage message"), 0}, {"program-name",OPT_PROGNAME, N_("NAME"), OPTION_HIDDEN, N_("set the program name"), 0}, {"HANG", OPT_HANG, N_("SECS"), OPTION_ARG_OPTIONAL | OPTION_HIDDEN, N_("hang for SECS seconds (default 3600)"), 0}, {NULL, 0, 0, 0, NULL, 0} }; static error_t argp_default_parser (int key, char *arg, struct argp_state *state) { switch (key) { case '?': __argp_state_help (state, state->out_stream, ARGP_HELP_STD_HELP); break; case OPT_USAGE: __argp_state_help (state, state->out_stream, ARGP_HELP_USAGE | ARGP_HELP_EXIT_OK); break; case OPT_PROGNAME: /* Set the program name. */ #if defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_NAME program_invocation_name = arg; #endif /* [Note that some systems only have PROGRAM_INVOCATION_SHORT_NAME (aka __PROGNAME), in which case, PROGRAM_INVOCATION_NAME is just defined to be that, so we have to be a bit careful here.] */ /* Update what we use for messages. */ state->name = __argp_base_name (arg); #if defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME program_invocation_short_name = state->name; #endif if ((state->flags & (ARGP_PARSE_ARGV0 | ARGP_NO_ERRS)) == ARGP_PARSE_ARGV0) /* Update what getopt uses too. */ state->argv[0] = arg; break; case OPT_HANG: _argp_hang = atoi (arg ? arg : "3600"); while (_argp_hang-- > 0) __sleep (1); break; default: return EBADKEY; } return 0; } static const struct argp argp_default_argp = {argp_default_options, &argp_default_parser, NULL, NULL, NULL, NULL, "libc"}; static const struct argp_option argp_version_options[] = { {"version", 'V', 0, 0, N_("print program version"), -1}, {NULL, 0, 0, 0, NULL, 0} }; static error_t argp_version_parser (int key, char *arg, struct argp_state *state) { switch (key) { case 'V': if (argp_program_version_hook) (*argp_program_version_hook) (state->out_stream, state); else if (argp_program_version) fprintf (state->out_stream, "%s\n", argp_program_version); else __argp_error (state, "%s", dgettext (state->root_argp->argp_domain, "(PROGRAM ERROR) No version known!?")); if (! (state->flags & ARGP_NO_EXIT)) exit (0); break; default: return EBADKEY; } return 0; } static const struct argp argp_version_argp = {argp_version_options, &argp_version_parser, NULL, NULL, NULL, NULL, "libc"}; /* Returns the offset into the getopt long options array LONG_OPTIONS of a long option with called NAME, or -1 if none is found. Passing NULL as NAME will return the number of options. */ static int find_long_option (struct option *long_options, const char *name) { struct option *l = long_options; while (l->name != NULL) if (name != NULL && strcmp (l->name, name) == 0) return l - long_options; else l++; if (name == NULL) return l - long_options; else return -1; } /* The state of a "group" during parsing. Each group corresponds to a particular argp structure from the tree of such descending from the top level argp passed to argp_parse. */ struct group { /* This group's parsing function. */ argp_parser_t parser; /* Which argp this group is from. */ const struct argp *argp; /* Points to the point in SHORT_OPTS corresponding to the end of the short options for this group. We use it to determine from which group a particular short options is from. */ char *short_end; /* The number of non-option args successfully handled by this parser. */ unsigned args_processed; /* This group's parser's parent's group. */ struct group *parent; unsigned parent_index; /* And the our position in the parent. */ /* These fields are swapped into and out of the state structure when calling this group's parser. */ void *input, **child_inputs; void *hook; }; /* Call GROUP's parser with KEY and ARG, swapping any group-specific info from STATE before calling, and back into state afterwards. If GROUP has no parser, EBADKEY is returned. */ static error_t group_parse (struct group *group, struct argp_state *state, int key, char *arg) { if (group->parser) { error_t err; state->hook = group->hook; state->input = group->input; state->child_inputs = group->child_inputs; state->arg_num = group->args_processed; err = (*group->parser)(key, arg, state); group->hook = state->hook; return err; } else return EBADKEY; } struct parser { const struct argp *argp; /* SHORT_OPTS is the getopt short options string for the union of all the groups of options. */ char *short_opts; /* LONG_OPTS is the array of getop long option structures for the union of all the groups of options. */ struct option *long_opts; /* OPT_DATA is the getopt data used for the re-entrant getopt. */ struct _getopt_data opt_data; /* States of the various parsing groups. */ struct group *groups; /* The end of the GROUPS array. */ struct group *egroup; /* A vector containing storage for the CHILD_INPUTS field in all groups. */ void **child_inputs; /* True if we think using getopt is still useful; if false, then remaining arguments are just passed verbatim with ARGP_KEY_ARG. This is cleared whenever getopt returns KEY_END, but may be set again if the user moves the next argument pointer backwards. */ int try_getopt; /* State block supplied to parsing routines. */ struct argp_state state; /* Memory used by this parser. */ void *storage; }; /* The next usable entries in the various parser tables being filled in by convert_options. */ struct parser_convert_state { struct parser *parser; char *short_end; struct option *long_end; void **child_inputs_end; }; /* Converts all options in ARGP (which is put in GROUP) and ancestors into getopt options stored in SHORT_OPTS and LONG_OPTS; SHORT_END and CVT->LONG_END are the points at which new options are added. Returns the next unused group entry. CVT holds state used during the conversion. */ static struct group * convert_options (const struct argp *argp, struct group *parent, unsigned parent_index, struct group *group, struct parser_convert_state *cvt) { /* REAL is the most recent non-alias value of OPT. */ const struct argp_option *real = argp->options; const struct argp_child *children = argp->children; if (real || argp->parser) { const struct argp_option *opt; if (real) for (opt = real; !__option_is_end (opt); opt++) { if (! (opt->flags & OPTION_ALIAS)) /* OPT isn't an alias, so we can use values from it. */ real = opt; if (! (real->flags & OPTION_DOC)) /* A real option (not just documentation). */ { if (__option_is_short (opt)) /* OPT can be used as a short option. */ { *cvt->short_end++ = opt->key; if (real->arg) { *cvt->short_end++ = ':'; if (real->flags & OPTION_ARG_OPTIONAL) *cvt->short_end++ = ':'; } *cvt->short_end = '\0'; /* keep 0 terminated */ } if (opt->name && find_long_option (cvt->parser->long_opts, opt->name) < 0) /* OPT can be used as a long option. */ { cvt->long_end->name = opt->name; cvt->long_end->has_arg = (real->arg ? (real->flags & OPTION_ARG_OPTIONAL ? optional_argument : required_argument) : no_argument); cvt->long_end->flag = 0; /* we add a disambiguating code to all the user's values (which is removed before we actually call the function to parse the value); this means that the user loses use of the high 8 bits in all his values (the sign of the lower bits is preserved however)... */ cvt->long_end->val = ((opt->key ? opt->key : real->key) & USER_MASK) + (((group - cvt->parser->groups) + 1) << USER_BITS); /* Keep the LONG_OPTS list terminated. */ (++cvt->long_end)->name = NULL; } } } group->parser = argp->parser; group->argp = argp; group->short_end = cvt->short_end; group->args_processed = 0; group->parent = parent; group->parent_index = parent_index; group->input = 0; group->hook = 0; group->child_inputs = 0; if (children) /* Assign GROUP's CHILD_INPUTS field some space from CVT->child_inputs_end.*/ { unsigned num_children = 0; while (children[num_children].argp) num_children++; group->child_inputs = cvt->child_inputs_end; cvt->child_inputs_end += num_children; } parent = group++; } else parent = 0; if (children) { unsigned index = 0; while (children->argp) group = convert_options (children++->argp, parent, index++, group, cvt); } return group; } /* Find the merged set of getopt options, with keys appropriately prefixed. */ static void parser_convert (struct parser *parser, const struct argp *argp, int flags) { struct parser_convert_state cvt; cvt.parser = parser; cvt.short_end = parser->short_opts; cvt.long_end = parser->long_opts; cvt.child_inputs_end = parser->child_inputs; if (flags & ARGP_IN_ORDER) *cvt.short_end++ = '-'; else if (flags & ARGP_NO_ARGS) *cvt.short_end++ = '+'; *cvt.short_end = '\0'; cvt.long_end->name = NULL; parser->argp = argp; if (argp) parser->egroup = convert_options (argp, 0, 0, parser->groups, &cvt); else parser->egroup = parser->groups; /* No parsers at all! */ } /* Lengths of various parser fields which we will allocated. */ struct parser_sizes { size_t short_len; /* Getopt short options string. */ size_t long_len; /* Getopt long options vector. */ size_t num_groups; /* Group structures we allocate. */ size_t num_child_inputs; /* Child input slots. */ }; /* For ARGP, increments the NUM_GROUPS field in SZS by the total number of argp structures descended from it, and the SHORT_LEN & LONG_LEN fields by the maximum lengths of the resulting merged getopt short options string and long-options array, respectively. */ static void calc_sizes (const struct argp *argp, struct parser_sizes *szs) { const struct argp_child *child = argp->children; const struct argp_option *opt = argp->options; if (opt || argp->parser) { szs->num_groups++; if (opt) { int num_opts = 0; while (!__option_is_end (opt++)) num_opts++; szs->short_len += num_opts * 3; /* opt + up to 2 ':'s */ szs->long_len += num_opts; } } if (child) while (child->argp) { calc_sizes ((child++)->argp, szs); szs->num_child_inputs++; } } /* Initializes PARSER to parse ARGP in a manner described by FLAGS. */ static error_t parser_init (struct parser *parser, const struct argp *argp, int argc, char **argv, int flags, void *input) { error_t err = 0; struct group *group; struct parser_sizes szs; struct _getopt_data opt_data = _GETOPT_DATA_INITIALIZER; char *storage; size_t glen, gsum; size_t clen, csum; size_t llen, lsum; size_t slen, ssum; szs.short_len = (flags & ARGP_NO_ARGS) ? 0 : 1; szs.long_len = 0; szs.num_groups = 0; szs.num_child_inputs = 0; if (argp) calc_sizes (argp, &szs); /* Lengths of the various bits of storage used by PARSER. */ glen = (szs.num_groups + 1) * sizeof (struct group); clen = szs.num_child_inputs * sizeof (void *); llen = (szs.long_len + 1) * sizeof (struct option); slen = szs.short_len + 1; /* Sums of previous lengths, properly aligned. There's no need to align gsum, since struct group is aligned at least as strictly as void * (since it contains a void * member). And there's no need to align lsum, since struct option is aligned at least as strictly as char. */ gsum = glen; csum = alignto (gsum + clen, alignof (struct option)); lsum = csum + llen; ssum = lsum + slen; parser->storage = malloc (ssum); if (! parser->storage) return ENOMEM; storage = parser->storage; parser->groups = parser->storage; parser->child_inputs = (void **) (storage + gsum); parser->long_opts = (struct option *) (storage + csum); parser->short_opts = storage + lsum; parser->opt_data = opt_data; memset (parser->child_inputs, 0, clen); parser_convert (parser, argp, flags); memset (&parser->state, 0, sizeof (struct argp_state)); parser->state.root_argp = parser->argp; parser->state.argc = argc; parser->state.argv = argv; parser->state.flags = flags; parser->state.err_stream = stderr; parser->state.out_stream = stdout; parser->state.next = 0; /* Tell getopt to initialize. */ parser->state.pstate = parser; parser->try_getopt = 1; /* Call each parser for the first time, giving it a chance to propagate values to child parsers. */ if (parser->groups < parser->egroup) parser->groups->input = input; for (group = parser->groups; group < parser->egroup && (!err || err == EBADKEY); group++) { if (group->parent) /* If a child parser, get the initial input value from the parent. */ group->input = group->parent->child_inputs[group->parent_index]; if (!group->parser && group->argp->children && group->argp->children->argp) /* For the special case where no parsing function is supplied for an argp, propagate its input to its first child, if any (this just makes very simple wrapper argps more convenient). */ group->child_inputs[0] = group->input; err = group_parse (group, &parser->state, ARGP_KEY_INIT, 0); } if (err == EBADKEY) err = 0; /* Some parser didn't understand. */ if (err) return err; if (parser->state.flags & ARGP_NO_ERRS) { parser->opt_data.opterr = 0; if (parser->state.flags & ARGP_PARSE_ARGV0) /* getopt always skips ARGV[0], so we have to fake it out. As long as OPTERR is 0, then it shouldn't actually try to access it. */ parser->state.argv--, parser->state.argc++; } else parser->opt_data.opterr = 1; /* Print error messages. */ if (parser->state.argv == argv && argv[0]) /* There's an argv[0]; use it for messages. */ parser->state.name = __argp_base_name (argv[0]); else parser->state.name = __argp_short_program_name (); return 0; } /* Free any storage consumed by PARSER (but not PARSER itself). */ static error_t parser_finalize (struct parser *parser, error_t err, int arg_ebadkey, int *end_index) { struct group *group; if (err == EBADKEY && arg_ebadkey) /* Suppress errors generated by unparsed arguments. */ err = 0; if (! err) { if (parser->state.next == parser->state.argc) /* We successfully parsed all arguments! Call all the parsers again, just a few more times... */ { for (group = parser->groups; group < parser->egroup && (!err || err==EBADKEY); group++) if (group->args_processed == 0) err = group_parse (group, &parser->state, ARGP_KEY_NO_ARGS, 0); for (group = parser->egroup - 1; group >= parser->groups && (!err || err==EBADKEY); group--) err = group_parse (group, &parser->state, ARGP_KEY_END, 0); if (err == EBADKEY) err = 0; /* Some parser didn't understand. */ /* Tell the user that all arguments are parsed. */ if (end_index) *end_index = parser->state.next; } else if (end_index) /* Return any remaining arguments to the user. */ *end_index = parser->state.next; else /* No way to return the remaining arguments, they must be bogus. */ { if (!(parser->state.flags & ARGP_NO_ERRS) && parser->state.err_stream) fprintf (parser->state.err_stream, dgettext (parser->argp->argp_domain, "%s: Too many arguments\n"), parser->state.name); err = EBADKEY; } } /* Okay, we're all done, with either an error or success; call the parsers to indicate which one. */ if (err) { /* Maybe print an error message. */ if (err == EBADKEY) /* An appropriate message describing what the error was should have been printed earlier. */ __argp_state_help (&parser->state, parser->state.err_stream, ARGP_HELP_STD_ERR); /* Since we didn't exit, give each parser an error indication. */ for (group = parser->groups; group < parser->egroup; group++) group_parse (group, &parser->state, ARGP_KEY_ERROR, 0); } else /* Notify parsers of success, and propagate back values from parsers. */ { /* We pass over the groups in reverse order so that child groups are given a chance to do there processing before passing back a value to the parent. */ for (group = parser->egroup - 1 ; group >= parser->groups && (!err || err == EBADKEY) ; group--) err = group_parse (group, &parser->state, ARGP_KEY_SUCCESS, 0); if (err == EBADKEY) err = 0; /* Some parser didn't understand. */ } /* Call parsers once more, to do any final cleanup. Errors are ignored. */ for (group = parser->egroup - 1; group >= parser->groups; group--) group_parse (group, &parser->state, ARGP_KEY_FINI, 0); if (err == EBADKEY) err = EINVAL; free (parser->storage); return err; } /* Call the user parsers to parse the non-option argument VAL, at the current position, returning any error. The state NEXT pointer is assumed to have been adjusted (by getopt) to point after this argument; this function will adjust it correctly to reflect however many args actually end up being consumed. */ static error_t parser_parse_arg (struct parser *parser, char *val) { /* Save the starting value of NEXT, first adjusting it so that the arg we're parsing is again the front of the arg vector. */ int index = --parser->state.next; error_t err = EBADKEY; struct group *group; int key = 0; /* Which of ARGP_KEY_ARG[S] we used. */ /* Try to parse the argument in each parser. */ for (group = parser->groups ; group < parser->egroup && err == EBADKEY ; group++) { parser->state.next++; /* For ARGP_KEY_ARG, consume the arg. */ key = ARGP_KEY_ARG; err = group_parse (group, &parser->state, key, val); if (err == EBADKEY) /* This parser doesn't like ARGP_KEY_ARG; try ARGP_KEY_ARGS instead. */ { parser->state.next--; /* For ARGP_KEY_ARGS, put back the arg. */ key = ARGP_KEY_ARGS; err = group_parse (group, &parser->state, key, 0); } } if (! err) { if (key == ARGP_KEY_ARGS) /* The default for ARGP_KEY_ARGS is to assume that if NEXT isn't changed by the user, *all* arguments should be considered consumed. */ parser->state.next = parser->state.argc; if (parser->state.next > index) /* Remember that we successfully processed a non-option argument -- but only if the user hasn't gotten tricky and set the clock back. */ (--group)->args_processed += (parser->state.next - index); else /* The user wants to reparse some args, give getopt another try. */ parser->try_getopt = 1; } return err; } /* Call the user parsers to parse the option OPT, with argument VAL, at the current position, returning any error. */ static error_t parser_parse_opt (struct parser *parser, int opt, char *val) { /* The group key encoded in the high bits; 0 for short opts or group_number + 1 for long opts. */ int group_key = opt >> USER_BITS; error_t err = EBADKEY; if (group_key == 0) /* A short option. By comparing OPT's position in SHORT_OPTS to the various starting positions in each group's SHORT_END field, we can determine which group OPT came from. */ { struct group *group; char *short_index = strchr (parser->short_opts, opt); if (short_index) for (group = parser->groups; group < parser->egroup; group++) if (group->short_end > short_index) { err = group_parse (group, &parser->state, opt, parser->opt_data.optarg); break; } } else /* A long option. Preserve the sign in the user key, without invoking undefined behavior. Assume two's complement. */ { int user_key = ((opt & (1 << (USER_BITS - 1))) ? ~USER_MASK : 0) | (opt & USER_MASK); err = group_parse (&parser->groups[group_key - 1], &parser->state, user_key, parser->opt_data.optarg); } if (err == EBADKEY) /* At least currently, an option not recognized is an error in the parser, because we pre-compute which parser is supposed to deal with each option. */ { static const char bad_key_err[] = N_("(PROGRAM ERROR) Option should have been recognized!?"); if (group_key == 0) __argp_error (&parser->state, "-%c: %s", opt, dgettext (parser->argp->argp_domain, bad_key_err)); else { struct option *long_opt = parser->long_opts; while (long_opt->val != opt && long_opt->name) long_opt++; __argp_error (&parser->state, "--%s: %s", long_opt->name ? long_opt->name : "???", dgettext (parser->argp->argp_domain, bad_key_err)); } } return err; } /* Parse the next argument in PARSER (as indicated by PARSER->state.next). Any error from the parsers is returned, and *ARGP_EBADKEY indicates whether a value of EBADKEY is due to an unrecognized argument (which is generally not fatal). */ static error_t parser_parse_next (struct parser *parser, int *arg_ebadkey) { int opt; error_t err = 0; if (parser->state.quoted && parser->state.next < parser->state.quoted) /* The next argument pointer has been moved to before the quoted region, so pretend we never saw the quoting "--", and give getopt another chance. If the user hasn't removed it, getopt will just process it again. */ parser->state.quoted = 0; if (parser->try_getopt && !parser->state.quoted) /* Give getopt a chance to parse this. */ { /* Put it back in OPTIND for getopt. */ parser->opt_data.optind = parser->state.next; /* Distinguish KEY_ERR from a real option. */ parser->opt_data.optopt = KEY_END; if (parser->state.flags & ARGP_LONG_ONLY) opt = _getopt_long_only_r (parser->state.argc, parser->state.argv, parser->short_opts, parser->long_opts, 0, &parser->opt_data); else opt = _getopt_long_r (parser->state.argc, parser->state.argv, parser->short_opts, parser->long_opts, 0, &parser->opt_data); /* And see what getopt did. */ parser->state.next = parser->opt_data.optind; if (opt == KEY_END) /* Getopt says there are no more options, so stop using getopt; we'll continue if necessary on our own. */ { parser->try_getopt = 0; if (parser->state.next > 1 && strcmp (parser->state.argv[parser->state.next - 1], QUOTE) == 0) /* Not only is this the end of the options, but it's a "quoted" region, which may have args that *look* like options, so we definitely shouldn't try to use getopt past here, whatever happens. */ parser->state.quoted = parser->state.next; } else if (opt == KEY_ERR && parser->opt_data.optopt != KEY_END) /* KEY_ERR can have the same value as a valid user short option, but in the case of a real error, getopt sets OPTOPT to the offending character, which can never be KEY_END. */ { *arg_ebadkey = 0; return EBADKEY; } } else opt = KEY_END; if (opt == KEY_END) { /* We're past what getopt considers the options. */ if (parser->state.next >= parser->state.argc || (parser->state.flags & ARGP_NO_ARGS)) /* Indicate that we're done. */ { *arg_ebadkey = 1; return EBADKEY; } else /* A non-option arg; simulate what getopt might have done. */ { opt = KEY_ARG; parser->opt_data.optarg = parser->state.argv[parser->state.next++]; } } if (opt == KEY_ARG) /* A non-option argument; try each parser in turn. */ err = parser_parse_arg (parser, parser->opt_data.optarg); else err = parser_parse_opt (parser, opt, parser->opt_data.optarg); if (err == EBADKEY) *arg_ebadkey = (opt == KEY_END || opt == KEY_ARG); return err; } /* Parse the options strings in ARGC & ARGV according to the argp in ARGP. FLAGS is one of the ARGP_ flags above. If END_INDEX is non-NULL, the index in ARGV of the first unparsed option is returned in it. If an unknown option is present, EINVAL is returned; if some parser routine returned a non-zero value, it is returned; otherwise 0 is returned. */ error_t __argp_parse (const struct argp *argp, int argc, char **argv, unsigned flags, int *end_index, void *input) { error_t err; struct parser parser; /* If true, then err == EBADKEY is a result of a non-option argument failing to be parsed (which in some cases isn't actually an error). */ int arg_ebadkey = 0; #ifndef _LIBC if (!(flags & ARGP_PARSE_ARGV0)) { #if HAVE_DECL_PROGRAM_INVOCATION_NAME if (!program_invocation_name) program_invocation_name = argv[0]; #endif #if HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME if (!program_invocation_short_name) program_invocation_short_name = __argp_base_name (argv[0]); #endif } #endif if (! (flags & ARGP_NO_HELP)) /* Add our own options. */ { struct argp_child *child = alloca (4 * sizeof (struct argp_child)); struct argp *top_argp = alloca (sizeof (struct argp)); /* TOP_ARGP has no options, it just serves to group the user & default argps. */ memset (top_argp, 0, sizeof (*top_argp)); top_argp->children = child; memset (child, 0, 4 * sizeof (struct argp_child)); if (argp) (child++)->argp = argp; (child++)->argp = &argp_default_argp; if (argp_program_version || argp_program_version_hook) (child++)->argp = &argp_version_argp; child->argp = 0; argp = top_argp; } /* Construct a parser for these arguments. */ err = parser_init (&parser, argp, argc, argv, flags, input); if (! err) /* Parse! */ { while (! err) err = parser_parse_next (&parser, &arg_ebadkey); err = parser_finalize (&parser, err, arg_ebadkey, end_index); } return err; } #ifdef weak_alias weak_alias (__argp_parse, argp_parse) #endif /* Return the input field for ARGP in the parser corresponding to STATE; used by the help routines. */ void * __argp_input (const struct argp *argp, const struct argp_state *state) { if (state) { struct group *group; struct parser *parser = state->pstate; for (group = parser->groups; group < parser->egroup; group++) if (group->argp == argp) return group->input; } return 0; } #ifdef weak_alias weak_alias (__argp_input, _argp_input) #endif gnuastro-0.5/bootstrapped/lib/argp-namefrob.h0000644000175000017500000001253413217200020016276 00000000000000/* Name frobnication for compiling argp outside of glibc Copyright (C) 1997-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #if !_LIBC /* This code is written for inclusion in gnu-libc, and uses names in the namespace reserved for libc. If we're not compiling in libc, define those names to be the normal ones instead. */ /* argp-parse functions */ #undef __argp_parse #define __argp_parse argp_parse #undef __option_is_end #define __option_is_end _option_is_end #undef __option_is_short #define __option_is_short _option_is_short #undef __argp_input #define __argp_input _argp_input /* argp-help functions */ #undef __argp_help #define __argp_help argp_help #undef __argp_error #define __argp_error argp_error #undef __argp_failure #define __argp_failure argp_failure #undef __argp_state_help #define __argp_state_help argp_state_help #undef __argp_usage #define __argp_usage argp_usage /* argp-fmtstream functions */ #undef __argp_make_fmtstream #define __argp_make_fmtstream argp_make_fmtstream #undef __argp_fmtstream_free #define __argp_fmtstream_free argp_fmtstream_free #undef __argp_fmtstream_putc #define __argp_fmtstream_putc argp_fmtstream_putc #undef __argp_fmtstream_puts #define __argp_fmtstream_puts argp_fmtstream_puts #undef __argp_fmtstream_write #define __argp_fmtstream_write argp_fmtstream_write #undef __argp_fmtstream_printf #define __argp_fmtstream_printf argp_fmtstream_printf #undef __argp_fmtstream_set_lmargin #define __argp_fmtstream_set_lmargin argp_fmtstream_set_lmargin #undef __argp_fmtstream_set_rmargin #define __argp_fmtstream_set_rmargin argp_fmtstream_set_rmargin #undef __argp_fmtstream_set_wmargin #define __argp_fmtstream_set_wmargin argp_fmtstream_set_wmargin #undef __argp_fmtstream_point #define __argp_fmtstream_point argp_fmtstream_point #undef __argp_fmtstream_update #define __argp_fmtstream_update _argp_fmtstream_update #undef __argp_fmtstream_ensure #define __argp_fmtstream_ensure _argp_fmtstream_ensure #undef __argp_fmtstream_lmargin #define __argp_fmtstream_lmargin argp_fmtstream_lmargin #undef __argp_fmtstream_rmargin #define __argp_fmtstream_rmargin argp_fmtstream_rmargin #undef __argp_fmtstream_wmargin #define __argp_fmtstream_wmargin argp_fmtstream_wmargin /* normal libc functions we call */ #undef __flockfile #define __flockfile flockfile #undef __funlockfile #define __funlockfile funlockfile #undef __mempcpy #define __mempcpy mempcpy #undef __sleep #define __sleep sleep #undef __strcasecmp #define __strcasecmp strcasecmp #undef __strchrnul #define __strchrnul strchrnul #undef __strerror_r #define __strerror_r strerror_r #undef __strndup #define __strndup strndup #undef __vsnprintf #define __vsnprintf vsnprintf #if defined(HAVE_DECL_CLEARERR_UNLOCKED) && !HAVE_DECL_CLEARERR_UNLOCKED # define clearerr_unlocked(x) clearerr (x) #endif #if defined(HAVE_DECL_FEOF_UNLOCKED) && !HAVE_DECL_FEOF_UNLOCKED # define feof_unlocked(x) feof (x) #endif #if defined(HAVE_DECL_FERROR_UNLOCKED) && !HAVE_DECL_FERROR_UNLOCKED # define ferror_unlocked(x) ferror (x) #endif #if defined(HAVE_DECL_FFLUSH_UNLOCKED) && !HAVE_DECL_FFLUSH_UNLOCKED # define fflush_unlocked(x) fflush (x) #endif #if defined(HAVE_DECL_FGETS_UNLOCKED) && !HAVE_DECL_FGETS_UNLOCKED # define fgets_unlocked(x,y,z) fgets (x,y,z) #endif #if defined(HAVE_DECL_FPUTC_UNLOCKED) && !HAVE_DECL_FPUTC_UNLOCKED # define fputc_unlocked(x,y) fputc (x,y) #endif #if defined(HAVE_DECL_FPUTS_UNLOCKED) && !HAVE_DECL_FPUTS_UNLOCKED # define fputs_unlocked(x,y) fputs (x,y) #endif #if defined(HAVE_DECL_FREAD_UNLOCKED) && !HAVE_DECL_FREAD_UNLOCKED # define fread_unlocked(w,x,y,z) fread (w,x,y,z) #endif #if defined(HAVE_DECL_FWRITE_UNLOCKED) && !HAVE_DECL_FWRITE_UNLOCKED # define fwrite_unlocked(w,x,y,z) fwrite (w,x,y,z) #endif #if defined(HAVE_DECL_GETC_UNLOCKED) && !HAVE_DECL_GETC_UNLOCKED # define getc_unlocked(x) getc (x) #endif #if defined(HAVE_DECL_GETCHAR_UNLOCKED) && !HAVE_DECL_GETCHAR_UNLOCKED # define getchar_unlocked() getchar () #endif #if defined(HAVE_DECL_PUTC_UNLOCKED) && !HAVE_DECL_PUTC_UNLOCKED # define putc_unlocked(x,y) putc (x,y) #endif #if defined(HAVE_DECL_PUTCHAR_UNLOCKED) && !HAVE_DECL_PUTCHAR_UNLOCKED # define putchar_unlocked(x) putchar (x) #endif #endif /* !_LIBC */ #ifndef __set_errno #define __set_errno(e) (errno = (e)) #endif #if defined GNULIB_ARGP_DISABLE_DIRNAME # define __argp_base_name(arg) arg #elif defined GNULIB_ARGP_EXTERN_BASENAME extern char *__argp_base_name (const char *arg); #else # include "dirname.h" # define __argp_base_name last_component #endif #if defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME # define __argp_short_program_name() (program_invocation_short_name) #else extern char *__argp_short_program_name (void); #endif gnuastro-0.5/bootstrapped/lib/argp-help.c0000644000175000017500000017225313217200020015435 00000000000000/* Hierarchical argument parsing help output Copyright (C) 1995-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _GNU_SOURCE # define _GNU_SOURCE 1 #endif #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include #include #include #include #include #ifdef _LIBC # include <../libio/libioP.h> # include #endif #ifdef _LIBC # include # undef dgettext # define dgettext(domain, msgid) \ __dcgettext (domain, msgid, LC_MESSAGES) #else # include "gettext.h" #endif #include "argp.h" #include "argp-fmtstream.h" #include "argp-namefrob.h" #ifndef SIZE_MAX # define SIZE_MAX ((size_t) -1) #endif /* User-selectable (using an environment variable) formatting parameters. These may be specified in an environment variable called 'ARGP_HELP_FMT', with a contents like: VAR1=VAL1,VAR2=VAL2,BOOLVAR2,no-BOOLVAR2 Where VALn must be a positive integer. The list of variables is in the UPARAM_NAMES vector, below. */ /* Default parameters. */ #define DUP_ARGS 0 /* True if option argument can be duplicated. */ #define DUP_ARGS_NOTE 1 /* True to print a note about duplicate args. */ #define SHORT_OPT_COL 2 /* column in which short options start */ #define LONG_OPT_COL 6 /* column in which long options start */ #define DOC_OPT_COL 2 /* column in which doc options start */ #define OPT_DOC_COL 29 /* column in which option text starts */ #define HEADER_COL 1 /* column in which group headers are printed */ #define USAGE_INDENT 12 /* indentation of wrapped usage lines */ #define RMARGIN 79 /* right margin used for wrapping */ /* User-selectable (using an environment variable) formatting parameters. They must all be of type 'int' for the parsing code to work. */ struct uparams { /* If true, arguments for an option are shown with both short and long options, even when a given option has both, e.g. '-x ARG, --longx=ARG'. If false, then if an option has both, the argument is only shown with the long one, e.g., '-x, --longx=ARG', and a message indicating that this really means both is printed below the options. */ int dup_args; /* This is true if when DUP_ARGS is false, and some duplicate arguments have been suppressed, an explanatory message should be printed. */ int dup_args_note; /* Various output columns. */ int short_opt_col; /* column in which short options start */ int long_opt_col; /* column in which long options start */ int doc_opt_col; /* column in which doc options start */ int opt_doc_col; /* column in which option text starts */ int header_col; /* column in which group headers are printed */ int usage_indent; /* indentation of wrapped usage lines */ int rmargin; /* right margin used for wrapping */ int valid; /* True when the values in here are valid. */ }; /* This is a global variable, as user options are only ever read once. */ static struct uparams uparams = { DUP_ARGS, DUP_ARGS_NOTE, SHORT_OPT_COL, LONG_OPT_COL, DOC_OPT_COL, OPT_DOC_COL, HEADER_COL, USAGE_INDENT, RMARGIN }; /* A particular uparam, and what the user name is. */ struct uparam_name { const char name[14]; /* User name. */ bool is_bool; /* Whether it's 'boolean'. */ unsigned char uparams_offs; /* Location of the (int) field in UPARAMS. */ }; /* The name-field mappings we know about. */ static const struct uparam_name uparam_names[] = { { "dup-args", true, offsetof (struct uparams, dup_args) }, { "dup-args-note", true, offsetof (struct uparams, dup_args_note) }, { "short-opt-col", false, offsetof (struct uparams, short_opt_col) }, { "long-opt-col", false, offsetof (struct uparams, long_opt_col) }, { "doc-opt-col", false, offsetof (struct uparams, doc_opt_col) }, { "opt-doc-col", false, offsetof (struct uparams, opt_doc_col) }, { "header-col", false, offsetof (struct uparams, header_col) }, { "usage-indent", false, offsetof (struct uparams, usage_indent) }, { "rmargin", false, offsetof (struct uparams, rmargin) } }; #define nuparam_names (sizeof (uparam_names) / sizeof (uparam_names[0])) static void validate_uparams (const struct argp_state *state, struct uparams *upptr) { const struct uparam_name *up; for (up = uparam_names; up < uparam_names + nuparam_names; up++) { if (up->is_bool || up->uparams_offs == offsetof (struct uparams, rmargin)) continue; if (*(int *)((char *)upptr + up->uparams_offs) >= upptr->rmargin) { __argp_failure (state, 0, 0, dgettext (state->root_argp->argp_domain, "\ ARGP_HELP_FMT: %s value is less than or equal to %s"), "rmargin", up->name); return; } } uparams = *upptr; uparams.valid = 1; } /* Read user options from the environment, and fill in UPARAMS appropriately. */ static void fill_in_uparams (const struct argp_state *state) { const char *var = getenv ("ARGP_HELP_FMT"); struct uparams new_params = uparams; #define SKIPWS(p) do { while (isspace ((unsigned char) *p)) p++; } while (0); if (var) { /* Parse var. */ while (*var) { SKIPWS (var); if (isalpha ((unsigned char) *var)) { size_t var_len; const struct uparam_name *un; int unspec = 0, val = 0; const char *arg = var; while (isalnum ((unsigned char) *arg) || *arg == '-' || *arg == '_') arg++; var_len = arg - var; SKIPWS (arg); if (*arg == '\0' || *arg == ',') unspec = 1; else if (*arg == '=') { arg++; SKIPWS (arg); } if (unspec) { if (var[0] == 'n' && var[1] == 'o' && var[2] == '-') { val = 0; var += 3; var_len -= 3; } else val = 1; } else if (isdigit ((unsigned char) *arg)) { val = atoi (arg); while (isdigit ((unsigned char) *arg)) arg++; SKIPWS (arg); } for (un = uparam_names; un < uparam_names + nuparam_names; un++) if (strlen (un->name) == var_len && strncmp (var, un->name, var_len) == 0) { if (unspec && !un->is_bool) __argp_failure (state, 0, 0, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "\ %.*s: ARGP_HELP_FMT parameter requires a value"), (int) var_len, var); else *(int *)((char *)&new_params + un->uparams_offs) = val; break; } if (un == uparam_names + nuparam_names) __argp_failure (state, 0, 0, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "\ %.*s: Unknown ARGP_HELP_FMT parameter"), (int) var_len, var); var = arg; if (*var == ',') var++; } else if (*var) { __argp_failure (state, 0, 0, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "Garbage in ARGP_HELP_FMT: %s"), var); break; } } validate_uparams (state, &new_params); } } /* Returns true if OPT hasn't been marked invisible. Visibility only affects whether OPT is displayed or used in sorting, not option shadowing. */ #define ovisible(opt) (! ((opt)->flags & OPTION_HIDDEN)) /* Returns true if OPT is an alias for an earlier option. */ #define oalias(opt) ((opt)->flags & OPTION_ALIAS) /* Returns true if OPT is a documentation-only entry. */ #define odoc(opt) ((opt)->flags & OPTION_DOC) /* Returns true if OPT should not be translated */ #define onotrans(opt) ((opt)->flags & OPTION_NO_TRANS) /* Returns true if OPT is the end-of-list marker for a list of options. */ #define oend(opt) __option_is_end (opt) /* Returns true if OPT has a short option. */ #define oshort(opt) __option_is_short (opt) /* The help format for a particular option is like: -xARG, -yARG, --long1=ARG, --long2=ARG Documentation... Where ARG will be omitted if there's no argument, for this option, or will be surrounded by "[" and "]" appropriately if the argument is optional. The documentation string is word-wrapped appropriately, and if the list of options is long enough, it will be started on a separate line. If there are no short options for a given option, the first long option is indented slightly in a way that's supposed to make most long options appear to be in a separate column. For example, the following output (from ps): -p PID, --pid=PID List the process PID --pgrp=PGRP List processes in the process group PGRP -P, -x, --no-parent Include processes without parents -Q, --all-fields Don't elide unusable fields (normally if there's some reason ps can't print a field for any process, it's removed from the output entirely) -r, --reverse, --gratuitously-long-reverse-option Reverse the order of any sort --session[=SID] Add the processes from the session SID (which defaults to the sid of the current process) Here are some more options: -f ZOT, --foonly=ZOT Glork a foonly -z, --zaza Snit a zar -?, --help Give this help list --usage Give a short usage message -V, --version Print program version The struct argp_option array for the above could look like: { {"pid", 'p', "PID", 0, "List the process PID"}, {"pgrp", OPT_PGRP, "PGRP", 0, "List processes in the process group PGRP"}, {"no-parent", 'P', 0, 0, "Include processes without parents"}, {0, 'x', 0, OPTION_ALIAS}, {"all-fields",'Q', 0, 0, "Don't elide unusable fields (normally" " if there's some reason ps can't" " print a field for any process, it's" " removed from the output entirely)" }, {"reverse", 'r', 0, 0, "Reverse the order of any sort"}, {"gratuitously-long-reverse-option", 0, 0, OPTION_ALIAS}, {"session", OPT_SESS, "SID", OPTION_ARG_OPTIONAL, "Add the processes from the session" " SID (which defaults to the sid of" " the current process)" }, {0,0,0,0, "Here are some more options:"}, {"foonly", 'f', "ZOT", 0, "Glork a foonly"}, {"zaza", 'z', 0, 0, "Snit a zar"}, {0} } Note that the last three options are automatically supplied by argp_parse, unless you tell it not to with ARGP_NO_HELP. */ /* Returns true if CH occurs between BEG and END. */ static int find_char (char ch, char *beg, char *end) { while (beg < end) if (*beg == ch) return 1; else beg++; return 0; } struct hol_cluster; /* fwd decl */ struct hol_entry { /* First option. */ const struct argp_option *opt; /* Number of options (including aliases). */ unsigned num; /* A pointers into the HOL's short_options field, to the first short option letter for this entry. The order of the characters following this point corresponds to the order of options pointed to by OPT, and there are at most NUM. A short option recorded in an option following OPT is only valid if it occurs in the right place in SHORT_OPTIONS (otherwise it's probably been shadowed by some other entry). */ char *short_options; /* Entries are sorted by their group first, in the order: 1, 2, ..., n, 0, -m, ..., -2, -1 and then alphabetically within each group. The default is 0. */ int group; /* The cluster of options this entry belongs to, or 0 if none. */ struct hol_cluster *cluster; /* The argp from which this option came. */ const struct argp *argp; /* Position in the array */ unsigned ord; }; /* A cluster of entries to reflect the argp tree structure. */ struct hol_cluster { /* A descriptive header printed before options in this cluster. */ const char *header; /* Used to order clusters within the same group with the same parent, according to the order in which they occurred in the parent argp's child list. */ int index; /* How to sort this cluster with respect to options and other clusters at the same depth (clusters always follow options in the same group). */ int group; /* The cluster to which this cluster belongs, or 0 if it's at the base level. */ struct hol_cluster *parent; /* The argp from which this cluster is (eventually) derived. */ const struct argp *argp; /* The distance this cluster is from the root. */ int depth; /* Clusters in a given hol are kept in a linked list, to make freeing them possible. */ struct hol_cluster *next; }; /* A list of options for help. */ struct hol { /* An array of hol_entry's. */ struct hol_entry *entries; /* The number of entries in this hol. If this field is zero, the others are undefined. */ unsigned num_entries; /* A string containing all short options in this HOL. Each entry contains pointers into this string, so the order can't be messed with blindly. */ char *short_options; /* Clusters of entries in this hol. */ struct hol_cluster *clusters; }; /* Create a struct hol from the options in ARGP. CLUSTER is the hol_cluster in which these entries occur, or 0, if at the root. */ static struct hol * make_hol (const struct argp *argp, struct hol_cluster *cluster) { char *so; const struct argp_option *o; const struct argp_option *opts = argp->options; struct hol_entry *entry; unsigned num_short_options = 0; struct hol *hol = malloc (sizeof (struct hol)); assert (hol); hol->num_entries = 0; hol->clusters = 0; if (opts) { int cur_group = 0; /* The first option must not be an alias. */ assert (! oalias (opts)); /* Calculate the space needed. */ for (o = opts; ! oend (o); o++) { if (! oalias (o)) hol->num_entries++; if (oshort (o)) num_short_options++; /* This is an upper bound. */ } hol->entries = malloc (sizeof (struct hol_entry) * hol->num_entries); hol->short_options = malloc (num_short_options + 1); assert (hol->entries && hol->short_options); if (SIZE_MAX <= UINT_MAX) assert (hol->num_entries <= SIZE_MAX / sizeof (struct hol_entry)); /* Fill in the entries. */ so = hol->short_options; for (o = opts, entry = hol->entries; ! oend (o); entry++) { entry->opt = o; entry->num = 0; entry->short_options = so; entry->group = cur_group = o->group ? o->group : ((!o->name && !o->key) ? cur_group + 1 : cur_group); entry->cluster = cluster; entry->argp = argp; do { entry->num++; if (oshort (o) && ! find_char (o->key, hol->short_options, so)) /* O has a valid short option which hasn't already been used.*/ *so++ = o->key; o++; } while (! oend (o) && oalias (o)); } *so = '\0'; /* null terminated so we can find the length */ } return hol; } /* Add a new cluster to HOL, with the given GROUP and HEADER (taken from the associated argp child list entry), INDEX, and PARENT, and return a pointer to it. ARGP is the argp that this cluster results from. */ static struct hol_cluster * hol_add_cluster (struct hol *hol, int group, const char *header, int index, struct hol_cluster *parent, const struct argp *argp) { struct hol_cluster *cl = malloc (sizeof (struct hol_cluster)); if (cl) { cl->group = group; cl->header = header; cl->index = index; cl->parent = parent; cl->argp = argp; cl->depth = parent ? parent->depth + 1 : 0; cl->next = hol->clusters; hol->clusters = cl; } return cl; } /* Free HOL and any resources it uses. */ static void hol_free (struct hol *hol) { struct hol_cluster *cl = hol->clusters; while (cl) { struct hol_cluster *next = cl->next; free (cl); cl = next; } if (hol->num_entries > 0) { free (hol->entries); free (hol->short_options); } free (hol); } static int hol_entry_short_iterate (const struct hol_entry *entry, int (*func)(const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie), const char *domain, void *cookie) { unsigned nopts; int val = 0; const struct argp_option *opt, *real = entry->opt; char *so = entry->short_options; for (opt = real, nopts = entry->num; nopts > 0 && !val; opt++, nopts--) if (oshort (opt) && *so == opt->key) { if (!oalias (opt)) real = opt; if (ovisible (opt)) val = (*func)(opt, real, domain, cookie); so++; } return val; } static inline int #if __GNUC__ >= 3 __attribute__ ((always_inline)) #endif hol_entry_long_iterate (const struct hol_entry *entry, int (*func)(const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie), const char *domain, void *cookie) { unsigned nopts; int val = 0; const struct argp_option *opt, *real = entry->opt; for (opt = real, nopts = entry->num; nopts > 0 && !val; opt++, nopts--) if (opt->name) { if (!oalias (opt)) real = opt; if (ovisible (opt)) val = (*func)(opt, real, domain, cookie); } return val; } /* Iterator that returns true for the first short option. */ static int until_short (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { return oshort (opt) ? opt->key : 0; } /* Returns the first valid short option in ENTRY, or 0 if there is none. */ static char hol_entry_first_short (const struct hol_entry *entry) { return hol_entry_short_iterate (entry, until_short, entry->argp->argp_domain, 0); } /* Returns the first valid long option in ENTRY, or 0 if there is none. */ static const char * hol_entry_first_long (const struct hol_entry *entry) { const struct argp_option *opt; unsigned num; for (opt = entry->opt, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) return opt->name; return 0; } /* Returns the entry in HOL with the long option name NAME, or 0 if there is none. */ static struct hol_entry * hol_find_entry (struct hol *hol, const char *name) { struct hol_entry *entry = hol->entries; unsigned num_entries = hol->num_entries; while (num_entries-- > 0) { const struct argp_option *opt = entry->opt; unsigned num_opts = entry->num; while (num_opts-- > 0) if (opt->name && ovisible (opt) && strcmp (opt->name, name) == 0) return entry; else opt++; entry++; } return 0; } /* If an entry with the long option NAME occurs in HOL, set its special sort position to GROUP. */ static void hol_set_group (struct hol *hol, const char *name, int group) { struct hol_entry *entry = hol_find_entry (hol, name); if (entry) entry->group = group; } /* Order by group: 0, 1, 2, ..., n, -m, ..., -2, -1. EQ is what to return if GROUP1 and GROUP2 are the same. */ static int group_cmp (int group1, int group2, int eq) { if (group1 == group2) return eq; else if ((group1 < 0 && group2 < 0) || (group1 >= 0 && group2 >= 0)) return group1 - group2; else return group2 - group1; } /* Compare clusters CL1 & CL2 by the order that they should appear in output. */ static int hol_cluster_cmp (const struct hol_cluster *cl1, const struct hol_cluster *cl2) { /* If one cluster is deeper than the other, use its ancestor at the same level, so that finding the common ancestor is straightforward. */ while (cl1->depth > cl2->depth) cl1 = cl1->parent; while (cl2->depth > cl1->depth) cl2 = cl2->parent; /* Now reduce both clusters to their ancestors at the point where both have a common parent; these can be directly compared. */ while (cl1->parent != cl2->parent) cl1 = cl1->parent, cl2 = cl2->parent; return group_cmp (cl1->group, cl2->group, cl2->index - cl1->index); } /* Return the ancestor of CL that's just below the root (i.e., has a parent of 0). */ static struct hol_cluster * hol_cluster_base (struct hol_cluster *cl) { while (cl->parent) cl = cl->parent; return cl; } /* Return true if CL1 is a child of CL2. */ static int hol_cluster_is_child (const struct hol_cluster *cl1, const struct hol_cluster *cl2) { while (cl1 && cl1 != cl2) cl1 = cl1->parent; return cl1 == cl2; } /* Given the name of an OPTION_DOC option, modifies NAME to start at the tail that should be used for comparisons, and returns true iff it should be treated as a non-option. */ static int canon_doc_option (const char **name) { int non_opt; /* Skip initial whitespace. */ while (isspace (**name)) (*name)++; /* Decide whether this looks like an option (leading '-') or not. */ non_opt = (**name != '-'); /* Skip until part of name used for sorting. */ while (**name && !isalnum (**name)) (*name)++; return non_opt; } #define HOL_ENTRY_PTRCMP(a,b) ((a)->ord < (b)->ord ? -1 : 1) /* Order ENTRY1 & ENTRY2 by the order which they should appear in a help listing. */ static int hol_entry_cmp (const struct hol_entry *entry1, const struct hol_entry *entry2) { /* The group numbers by which the entries should be ordered; if either is in a cluster, then this is just the group within the cluster. */ int group1 = entry1->group, group2 = entry2->group; if (entry1->cluster != entry2->cluster) { /* The entries are not within the same cluster, so we can't compare them directly, we have to use the appropriate clustering level too. */ if (! entry1->cluster) /* ENTRY1 is at the 'base level', not in a cluster, so we have to compare it's group number with that of the base cluster in which ENTRY2 resides. Note that if they're in the same group, the clustered option always comes last. */ return group_cmp (group1, hol_cluster_base (entry2->cluster)->group, -1); else if (! entry2->cluster) /* Likewise, but ENTRY2's not in a cluster. */ return group_cmp (hol_cluster_base (entry1->cluster)->group, group2, 1); else /* Both entries are in clusters, we can just compare the clusters. */ return hol_cluster_cmp (entry1->cluster, entry2->cluster); } else if (group1 == group2) /* The entries are both in the same cluster and group, so compare them alphabetically. */ { int short1 = hol_entry_first_short (entry1); int short2 = hol_entry_first_short (entry2); int doc1 = odoc (entry1->opt); int doc2 = odoc (entry2->opt); const char *long1 = hol_entry_first_long (entry1); const char *long2 = hol_entry_first_long (entry2); if (doc1) doc1 = long1 != NULL && canon_doc_option (&long1); if (doc2) doc2 = long2 != NULL && canon_doc_option (&long2); if (doc1 != doc2) /* 'documentation' options always follow normal options (or documentation options that *look* like normal options). */ return doc1 - doc2; else if (!short1 && !short2 && long1 && long2) /* Only long options. */ return __strcasecmp (long1, long2); else /* Compare short/short, long/short, short/long, using the first character of long options. Entries without *any* valid options (such as options with OPTION_HIDDEN set) will be put first, but as they're not displayed, it doesn't matter where they are. */ { char first1 = short1 ? short1 : long1 ? *long1 : 0; char first2 = short2 ? short2 : long2 ? *long2 : 0; #ifdef _tolower int lower_cmp = _tolower (first1) - _tolower (first2); #else int lower_cmp = tolower (first1) - tolower (first2); #endif /* Compare ignoring case, except when the options are both the same letter, in which case lower-case always comes first. */ return lower_cmp ? lower_cmp : first2 - first1; } } else /* Within the same cluster, but not the same group, so just compare groups. */ return group_cmp (group1, group2, 0); } /* Version of hol_entry_cmp with correct signature for qsort. */ static int hol_entry_qcmp (const void *entry1_v, const void *entry2_v) { return hol_entry_cmp (entry1_v, entry2_v); } /* Sort HOL by group and alphabetically by option name (with short options taking precedence over long). Since the sorting is for display purposes only, the shadowing of options isn't effected. */ static void hol_sort (struct hol *hol) { if (hol->num_entries > 0) { unsigned i; struct hol_entry *e; for (i = 0, e = hol->entries; i < hol->num_entries; i++, e++) e->ord = i; qsort (hol->entries, hol->num_entries, sizeof (struct hol_entry), hol_entry_qcmp); } } /* Append MORE to HOL, destroying MORE in the process. Options in HOL shadow any in MORE with the same name. */ static void hol_append (struct hol *hol, struct hol *more) { struct hol_cluster **cl_end = &hol->clusters; /* Steal MORE's cluster list, and add it to the end of HOL's. */ while (*cl_end) cl_end = &(*cl_end)->next; *cl_end = more->clusters; more->clusters = 0; /* Merge entries. */ if (more->num_entries > 0) { if (hol->num_entries == 0) { hol->num_entries = more->num_entries; hol->entries = more->entries; hol->short_options = more->short_options; more->num_entries = 0; /* Mark MORE's fields as invalid. */ } else /* Append the entries in MORE to those in HOL, taking care to only add non-shadowed SHORT_OPTIONS values. */ { unsigned left; char *so, *more_so; struct hol_entry *e; unsigned num_entries = hol->num_entries + more->num_entries; struct hol_entry *entries = malloc (num_entries * sizeof (struct hol_entry)); unsigned hol_so_len = strlen (hol->short_options); char *short_options = malloc (hol_so_len + strlen (more->short_options) + 1); assert (entries && short_options); if (SIZE_MAX <= UINT_MAX) assert (num_entries <= SIZE_MAX / sizeof (struct hol_entry)); __mempcpy (__mempcpy (entries, hol->entries, hol->num_entries * sizeof (struct hol_entry)), more->entries, more->num_entries * sizeof (struct hol_entry)); __mempcpy (short_options, hol->short_options, hol_so_len); /* Fix up the short options pointers from HOL. */ for (e = entries, left = hol->num_entries; left > 0; e++, left--) e->short_options = short_options + (e->short_options - hol->short_options); /* Now add the short options from MORE, fixing up its entries too. */ so = short_options + hol_so_len; more_so = more->short_options; for (left = more->num_entries; left > 0; e++, left--) { int opts_left; const struct argp_option *opt; e->short_options = so; for (opts_left = e->num, opt = e->opt; opts_left; opt++, opts_left--) { int ch = *more_so; if (oshort (opt) && ch == opt->key) /* The next short option in MORE_SO, CH, is from OPT. */ { if (! find_char (ch, short_options, short_options + hol_so_len)) /* The short option CH isn't shadowed by HOL's options, so add it to the sum. */ *so++ = ch; more_so++; } } } *so = '\0'; free (hol->entries); free (hol->short_options); hol->entries = entries; hol->num_entries = num_entries; hol->short_options = short_options; } } hol_free (more); } /* Inserts enough spaces to make sure STREAM is at column COL. */ static void indent_to (argp_fmtstream_t stream, unsigned col) { int needed = col - __argp_fmtstream_point (stream); while (needed-- > 0) __argp_fmtstream_putc (stream, ' '); } /* Output to STREAM either a space, or a newline if there isn't room for at least ENSURE characters before the right margin. */ static void space (argp_fmtstream_t stream, size_t ensure) { if (__argp_fmtstream_point (stream) + ensure >= __argp_fmtstream_rmargin (stream)) __argp_fmtstream_putc (stream, '\n'); else __argp_fmtstream_putc (stream, ' '); } /* If the option REAL has an argument, we print it in using the printf format REQ_FMT or OPT_FMT depending on whether it's a required or optional argument. */ static void arg (const struct argp_option *real, const char *req_fmt, const char *opt_fmt, const char *domain, argp_fmtstream_t stream) { if (real->arg) { if (real->flags & OPTION_ARG_OPTIONAL) __argp_fmtstream_printf (stream, opt_fmt, dgettext (domain, real->arg)); else __argp_fmtstream_printf (stream, req_fmt, dgettext (domain, real->arg)); } } /* Helper functions for hol_entry_help. */ /* State used during the execution of hol_help. */ struct hol_help_state { /* PREV_ENTRY should contain the previous entry printed, or 0. */ struct hol_entry *prev_entry; /* If an entry is in a different group from the previous one, and SEP_GROUPS is true, then a blank line will be printed before any output. */ int sep_groups; /* True if a duplicate option argument was suppressed (only ever set if UPARAMS.dup_args is false). */ int suppressed_dup_arg; }; /* Some state used while printing a help entry (used to communicate with helper functions). See the doc for hol_entry_help for more info, as most of the fields are copied from its arguments. */ struct pentry_state { const struct hol_entry *entry; argp_fmtstream_t stream; struct hol_help_state *hhstate; /* True if nothing's been printed so far. */ int first; /* If non-zero, the state that was used to print this help. */ const struct argp_state *state; }; /* If a user doc filter should be applied to DOC, do so. */ static const char * filter_doc (const char *doc, int key, const struct argp *argp, const struct argp_state *state) { if (argp && argp->help_filter) /* We must apply a user filter to this output. */ { void *input = __argp_input (argp, state); return (*argp->help_filter) (key, doc, input); } else /* No filter. */ return doc; } /* Prints STR as a header line, with the margin lines set appropriately, and notes the fact that groups should be separated with a blank line. ARGP is the argp that should dictate any user doc filtering to take place. Note that the previous wrap margin isn't restored, but the left margin is reset to 0. */ static void print_header (const char *str, const struct argp *argp, struct pentry_state *pest) { const char *tstr = dgettext (argp->argp_domain, str); const char *fstr = filter_doc (tstr, ARGP_KEY_HELP_HEADER, argp, pest->state); if (fstr) { if (*fstr) { if (pest->hhstate->prev_entry) /* Precede with a blank line. */ __argp_fmtstream_putc (pest->stream, '\n'); indent_to (pest->stream, uparams.header_col); __argp_fmtstream_set_lmargin (pest->stream, uparams.header_col); __argp_fmtstream_set_wmargin (pest->stream, uparams.header_col); __argp_fmtstream_puts (pest->stream, fstr); __argp_fmtstream_set_lmargin (pest->stream, 0); __argp_fmtstream_putc (pest->stream, '\n'); } pest->hhstate->sep_groups = 1; /* Separate subsequent groups. */ } if (fstr != tstr) free ((char *) fstr); } /* Inserts a comma if this isn't the first item on the line, and then makes sure we're at least to column COL. If this *is* the first item on a line, prints any pending whitespace/headers that should precede this line. Also clears FIRST. */ static void comma (unsigned col, struct pentry_state *pest) { if (pest->first) { const struct hol_entry *pe = pest->hhstate->prev_entry; const struct hol_cluster *cl = pest->entry->cluster; if (pest->hhstate->sep_groups && pe && pest->entry->group != pe->group) __argp_fmtstream_putc (pest->stream, '\n'); if (cl && cl->header && *cl->header && (!pe || (pe->cluster != cl && !hol_cluster_is_child (pe->cluster, cl)))) /* If we're changing clusters, then this must be the start of the ENTRY's cluster unless that is an ancestor of the previous one (in which case we had just popped into a sub-cluster for a bit). If so, then print the cluster's header line. */ { int old_wm = __argp_fmtstream_wmargin (pest->stream); print_header (cl->header, cl->argp, pest); __argp_fmtstream_set_wmargin (pest->stream, old_wm); } pest->first = 0; } else __argp_fmtstream_puts (pest->stream, ", "); indent_to (pest->stream, col); } /* Print help for ENTRY to STREAM. */ static void hol_entry_help (struct hol_entry *entry, const struct argp_state *state, argp_fmtstream_t stream, struct hol_help_state *hhstate) { unsigned num; const struct argp_option *real = entry->opt, *opt; char *so = entry->short_options; int have_long_opt = 0; /* We have any long options. */ /* Saved margins. */ int old_lm = __argp_fmtstream_set_lmargin (stream, 0); int old_wm = __argp_fmtstream_wmargin (stream); /* PEST is a state block holding some of our variables that we'd like to share with helper functions. */ struct pentry_state pest = { entry, stream, hhstate, 1, state }; if (! odoc (real)) for (opt = real, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) { have_long_opt = 1; break; } /* First emit short options. */ __argp_fmtstream_set_wmargin (stream, uparams.short_opt_col); /* For truly bizarre cases. */ for (opt = real, num = entry->num; num > 0; opt++, num--) if (oshort (opt) && opt->key == *so) /* OPT has a valid (non shadowed) short option. */ { if (ovisible (opt)) { comma (uparams.short_opt_col, &pest); __argp_fmtstream_putc (stream, '-'); __argp_fmtstream_putc (stream, *so); if (!have_long_opt || uparams.dup_args) arg (real, " %s", "[%s]", state == NULL ? NULL : state->root_argp->argp_domain, stream); else if (real->arg) hhstate->suppressed_dup_arg = 1; } so++; } /* Now, long options. */ if (odoc (real)) /* A "documentation" option. */ { __argp_fmtstream_set_wmargin (stream, uparams.doc_opt_col); for (opt = real, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) { comma (uparams.doc_opt_col, &pest); /* Calling dgettext here isn't quite right, since sorting will have been done on the original; but documentation options should be pretty rare anyway... */ __argp_fmtstream_puts (stream, dgettext (state == NULL ? NULL : state->root_argp->argp_domain, opt->name)); } } else /* A real long option. */ { __argp_fmtstream_set_wmargin (stream, uparams.long_opt_col); for (opt = real, num = entry->num; num > 0; opt++, num--) if (opt->name && ovisible (opt)) { comma (uparams.long_opt_col, &pest); __argp_fmtstream_printf (stream, "--%s", opt->name); arg (real, "=%s", "[=%s]", state == NULL ? NULL : state->root_argp->argp_domain, stream); } } /* Next, documentation strings. */ __argp_fmtstream_set_lmargin (stream, 0); if (pest.first) { /* Didn't print any switches, what's up? */ if (!oshort (real) && !real->name) /* This is a group header, print it nicely. */ print_header (real->doc, entry->argp, &pest); else /* Just a totally shadowed option or null header; print nothing. */ goto cleanup; /* Just return, after cleaning up. */ } else { const char *tstr = real->doc ? dgettext (state == NULL ? NULL : state->root_argp->argp_domain, real->doc) : 0; const char *fstr = filter_doc (tstr, real->key, entry->argp, state); if (fstr && *fstr) { unsigned int col = __argp_fmtstream_point (stream); __argp_fmtstream_set_lmargin (stream, uparams.opt_doc_col); __argp_fmtstream_set_wmargin (stream, uparams.opt_doc_col); if (col > (unsigned int) (uparams.opt_doc_col + 3)) __argp_fmtstream_putc (stream, '\n'); else if (col >= (unsigned int) uparams.opt_doc_col) __argp_fmtstream_puts (stream, " "); else indent_to (stream, uparams.opt_doc_col); __argp_fmtstream_puts (stream, fstr); } if (fstr && fstr != tstr) free ((char *) fstr); /* Reset the left margin. */ __argp_fmtstream_set_lmargin (stream, 0); __argp_fmtstream_putc (stream, '\n'); } hhstate->prev_entry = entry; cleanup: __argp_fmtstream_set_lmargin (stream, old_lm); __argp_fmtstream_set_wmargin (stream, old_wm); } /* Output a long help message about the options in HOL to STREAM. */ static void hol_help (struct hol *hol, const struct argp_state *state, argp_fmtstream_t stream) { unsigned num; struct hol_entry *entry; struct hol_help_state hhstate = { 0, 0, 0 }; for (entry = hol->entries, num = hol->num_entries; num > 0; entry++, num--) hol_entry_help (entry, state, stream, &hhstate); if (hhstate.suppressed_dup_arg && uparams.dup_args_note) { const char *tstr = dgettext (state == NULL ? NULL : state->root_argp->argp_domain, "\ Mandatory or optional arguments to long options are also mandatory or \ optional for any corresponding short options."); const char *fstr = filter_doc (tstr, ARGP_KEY_HELP_DUP_ARGS_NOTE, state ? state->root_argp : 0, state); if (fstr && *fstr) { __argp_fmtstream_putc (stream, '\n'); __argp_fmtstream_puts (stream, fstr); __argp_fmtstream_putc (stream, '\n'); } if (fstr && fstr != tstr) free ((char *) fstr); } } /* Helper functions for hol_usage. */ /* If OPT is a short option without an arg, append its key to the string pointer pointer to by COOKIE, and advance the pointer. */ static int add_argless_short_opt (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { char **snao_end = cookie; if (!(opt->arg || real->arg) && !((opt->flags | real->flags) & OPTION_NO_USAGE)) *(*snao_end)++ = opt->key; return 0; } /* If OPT is a short option with an arg, output a usage entry for it to the stream pointed at by COOKIE. */ static int usage_argful_short_opt (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { argp_fmtstream_t stream = cookie; const char *arg = opt->arg; int flags = opt->flags | real->flags; if (! arg) arg = real->arg; if (arg && !(flags & OPTION_NO_USAGE)) { arg = dgettext (domain, arg); if (flags & OPTION_ARG_OPTIONAL) __argp_fmtstream_printf (stream, " [-%c[%s]]", opt->key, arg); else { /* Manually do line wrapping so that it (probably) won't get wrapped at the embedded space. */ space (stream, 6 + strlen (arg)); __argp_fmtstream_printf (stream, "[-%c %s]", opt->key, arg); } } return 0; } /* Output a usage entry for the long option opt to the stream pointed at by COOKIE. */ static int usage_long_opt (const struct argp_option *opt, const struct argp_option *real, const char *domain, void *cookie) { argp_fmtstream_t stream = cookie; const char *arg = opt->arg; int flags = opt->flags | real->flags; if (! arg) arg = real->arg; if (! (flags & OPTION_NO_USAGE)) { if (arg) { arg = dgettext (domain, arg); if (flags & OPTION_ARG_OPTIONAL) __argp_fmtstream_printf (stream, " [--%s[=%s]]", opt->name, arg); else __argp_fmtstream_printf (stream, " [--%s=%s]", opt->name, arg); } else __argp_fmtstream_printf (stream, " [--%s]", opt->name); } return 0; } /* Print a short usage description for the arguments in HOL to STREAM. */ static void hol_usage (struct hol *hol, argp_fmtstream_t stream) { if (hol->num_entries > 0) { unsigned nentries; struct hol_entry *entry; char *short_no_arg_opts = alloca (strlen (hol->short_options) + 1); char *snao_end = short_no_arg_opts; /* First we put a list of short options without arguments. */ for (entry = hol->entries, nentries = hol->num_entries ; nentries > 0 ; entry++, nentries--) hol_entry_short_iterate (entry, add_argless_short_opt, entry->argp->argp_domain, &snao_end); if (snao_end > short_no_arg_opts) { *snao_end++ = 0; __argp_fmtstream_printf (stream, " [-%s]", short_no_arg_opts); } /* Now a list of short options *with* arguments. */ for (entry = hol->entries, nentries = hol->num_entries ; nentries > 0 ; entry++, nentries--) hol_entry_short_iterate (entry, usage_argful_short_opt, entry->argp->argp_domain, stream); /* Finally, a list of long options (whew!). */ for (entry = hol->entries, nentries = hol->num_entries ; nentries > 0 ; entry++, nentries--) hol_entry_long_iterate (entry, usage_long_opt, entry->argp->argp_domain, stream); } } /* Make a HOL containing all levels of options in ARGP. CLUSTER is the cluster in which ARGP's entries should be clustered, or 0. */ static struct hol * argp_hol (const struct argp *argp, struct hol_cluster *cluster) { const struct argp_child *child = argp->children; struct hol *hol = make_hol (argp, cluster); if (child) while (child->argp) { struct hol_cluster *child_cluster = ((child->group || child->header) /* Put CHILD->argp within its own cluster. */ ? hol_add_cluster (hol, child->group, child->header, child - argp->children, cluster, argp) /* Just merge it into the parent's cluster. */ : cluster); hol_append (hol, argp_hol (child->argp, child_cluster)) ; child++; } return hol; } /* Calculate how many different levels with alternative args strings exist in ARGP. */ static size_t argp_args_levels (const struct argp *argp) { size_t levels = 0; const struct argp_child *child = argp->children; if (argp->args_doc && strchr (argp->args_doc, '\n')) levels++; if (child) while (child->argp) levels += argp_args_levels ((child++)->argp); return levels; } /* Print all the non-option args documented in ARGP to STREAM. Any output is preceded by a space. LEVELS is a pointer to a byte vector the length returned by argp_args_levels; it should be initialized to zero, and updated by this routine for the next call if ADVANCE is true. True is returned as long as there are more patterns to output. */ static int argp_args_usage (const struct argp *argp, const struct argp_state *state, char **levels, int advance, argp_fmtstream_t stream) { char *our_level = *levels; int multiple = 0; const struct argp_child *child = argp->children; const char *tdoc = dgettext (argp->argp_domain, argp->args_doc), *nl = 0; const char *fdoc = filter_doc (tdoc, ARGP_KEY_HELP_ARGS_DOC, argp, state); if (fdoc) { const char *cp = fdoc; nl = __strchrnul (cp, '\n'); if (*nl != '\0') /* This is a 'multi-level' args doc; advance to the correct position as determined by our state in LEVELS, and update LEVELS. */ { int i; multiple = 1; for (i = 0; i < *our_level; i++) cp = nl + 1, nl = __strchrnul (cp, '\n'); (*levels)++; } /* Manually do line wrapping so that it (probably) won't get wrapped at any embedded spaces. */ space (stream, 1 + nl - cp); __argp_fmtstream_write (stream, cp, nl - cp); } if (fdoc && fdoc != tdoc) free ((char *)fdoc); /* Free user's modified doc string. */ if (child) while (child->argp) advance = !argp_args_usage ((child++)->argp, state, levels, advance, stream); if (advance && multiple) { /* Need to increment our level. */ if (*nl) /* There's more we can do here. */ { (*our_level)++; advance = 0; /* Our parent shouldn't advance also. */ } else if (*our_level > 0) /* We had multiple levels, but used them up; reset to zero. */ *our_level = 0; } return !advance; } /* Print the documentation for ARGP to STREAM; if POST is false, then everything preceding a '\v' character in the documentation strings (or the whole string, for those with none) is printed, otherwise, everything following the '\v' character (nothing for strings without). Each separate bit of documentation is separated a blank line, and if PRE_BLANK is true, then the first is as well. If FIRST_ONLY is true, only the first occurrence is output. Returns true if anything was output. */ static int argp_doc (const struct argp *argp, const struct argp_state *state, int post, int pre_blank, int first_only, argp_fmtstream_t stream) { const char *text; const char *inp_text; void *input = 0; int anything = 0; size_t inp_text_limit = 0; const char *doc = dgettext (argp->argp_domain, argp->doc); const struct argp_child *child = argp->children; if (doc) { char *vt = strchr (doc, '\v'); inp_text = post ? (vt ? vt + 1 : 0) : doc; inp_text_limit = (!post && vt) ? (vt - doc) : 0; } else inp_text = 0; if (argp->help_filter) /* We have to filter the doc strings. */ { if (inp_text_limit) /* Copy INP_TEXT so that it's nul-terminated. */ inp_text = __strndup (inp_text, inp_text_limit); input = __argp_input (argp, state); text = (*argp->help_filter) (post ? ARGP_KEY_HELP_POST_DOC : ARGP_KEY_HELP_PRE_DOC, inp_text, input); } else text = (const char *) inp_text; if (text) { if (pre_blank) __argp_fmtstream_putc (stream, '\n'); if (text == inp_text && inp_text_limit) __argp_fmtstream_write (stream, inp_text, inp_text_limit); else __argp_fmtstream_puts (stream, text); if (__argp_fmtstream_point (stream) > __argp_fmtstream_lmargin (stream)) __argp_fmtstream_putc (stream, '\n'); anything = 1; } if (text && text != inp_text) free ((char *) text); /* Free TEXT returned from the help filter. */ if (inp_text && inp_text_limit && argp->help_filter) free ((char *) inp_text); /* We copied INP_TEXT, so free it now. */ if (post && argp->help_filter) /* Now see if we have to output a ARGP_KEY_HELP_EXTRA text. */ { text = (*argp->help_filter) (ARGP_KEY_HELP_EXTRA, 0, input); if (text) { if (anything || pre_blank) __argp_fmtstream_putc (stream, '\n'); __argp_fmtstream_puts (stream, text); free ((char *) text); if (__argp_fmtstream_point (stream) > __argp_fmtstream_lmargin (stream)) __argp_fmtstream_putc (stream, '\n'); anything = 1; } } if (child) while (child->argp && !(first_only && anything)) anything |= argp_doc ((child++)->argp, state, post, anything || pre_blank, first_only, stream); return anything; } /* Output a usage message for ARGP to STREAM. If called from argp_state_help, STATE is the relevent parsing state. FLAGS are from the set ARGP_HELP_*. NAME is what to use wherever a 'program name' is needed. */ static void _help (const struct argp *argp, const struct argp_state *state, FILE *stream, unsigned flags, char *name) { int anything = 0; /* Whether we've output anything. */ struct hol *hol = 0; argp_fmtstream_t fs; if (! stream) return; #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __flockfile (stream); #endif if (! uparams.valid) fill_in_uparams (state); fs = __argp_make_fmtstream (stream, 0, uparams.rmargin, 0); if (! fs) { #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif return; } if (flags & (ARGP_HELP_USAGE | ARGP_HELP_SHORT_USAGE | ARGP_HELP_LONG)) { hol = argp_hol (argp, 0); /* If present, these options always come last. */ hol_set_group (hol, "help", -1); hol_set_group (hol, "version", -1); hol_sort (hol); } if (flags & (ARGP_HELP_USAGE | ARGP_HELP_SHORT_USAGE)) /* Print a short "Usage:" message. */ { int first_pattern = 1, more_patterns; size_t num_pattern_levels = argp_args_levels (argp); char *pattern_levels = alloca (num_pattern_levels); memset (pattern_levels, 0, num_pattern_levels); do { int old_lm; int old_wm = __argp_fmtstream_set_wmargin (fs, uparams.usage_indent); char *levels = pattern_levels; if (first_pattern) __argp_fmtstream_printf (fs, "%s %s", dgettext (argp->argp_domain, "Usage:"), name); else __argp_fmtstream_printf (fs, "%s %s", dgettext (argp->argp_domain, " or: "), name); /* We set the lmargin as well as the wmargin, because hol_usage manually wraps options with newline to avoid annoying breaks. */ old_lm = __argp_fmtstream_set_lmargin (fs, uparams.usage_indent); if (flags & ARGP_HELP_SHORT_USAGE) /* Just show where the options go. */ { if (hol->num_entries > 0) __argp_fmtstream_puts (fs, dgettext (argp->argp_domain, " [OPTION...]")); } else /* Actually print the options. */ { hol_usage (hol, fs); flags |= ARGP_HELP_SHORT_USAGE; /* But only do so once. */ } more_patterns = argp_args_usage (argp, state, &levels, 1, fs); __argp_fmtstream_set_wmargin (fs, old_wm); __argp_fmtstream_set_lmargin (fs, old_lm); __argp_fmtstream_putc (fs, '\n'); anything = 1; first_pattern = 0; } while (more_patterns); } if (flags & ARGP_HELP_PRE_DOC) anything |= argp_doc (argp, state, 0, 0, 1, fs); if (flags & ARGP_HELP_SEE) { __argp_fmtstream_printf (fs, dgettext (argp->argp_domain, "\ Try '%s --help' or '%s --usage' for more information.\n"), name, name); anything = 1; } if (flags & ARGP_HELP_LONG) /* Print a long, detailed help message. */ { /* Print info about all the options. */ if (hol->num_entries > 0) { if (anything) __argp_fmtstream_putc (fs, '\n'); hol_help (hol, state, fs); anything = 1; } } if (flags & ARGP_HELP_POST_DOC) /* Print any documentation strings at the end. */ anything |= argp_doc (argp, state, 1, anything, 0, fs); if ((flags & ARGP_HELP_BUG_ADDR) && argp_program_bug_address) { if (anything) __argp_fmtstream_putc (fs, '\n'); __argp_fmtstream_printf (fs, dgettext (argp->argp_domain, "Report bugs to %s.\n"), argp_program_bug_address); anything = 1; } #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif if (hol) hol_free (hol); __argp_fmtstream_free (fs); } /* Output a usage message for ARGP to STREAM. FLAGS are from the set ARGP_HELP_*. NAME is what to use wherever a 'program name' is needed. */ void __argp_help (const struct argp *argp, FILE *stream, unsigned flags, char *name) { _help (argp, 0, stream, flags, name); } #ifdef weak_alias weak_alias (__argp_help, argp_help) #endif #if ! (defined _LIBC || HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME) char * __argp_short_program_name (void) { # if HAVE_DECL_PROGRAM_INVOCATION_NAME char *name = strrchr (program_invocation_name, '/'); return name ? name + 1 : program_invocation_name; # else /* FIXME: What now? Miles suggests that it is better to use NULL, but currently the value is passed on directly to fputs_unlocked, so that requires more changes. */ # if __GNUC__ # warning No reasonable value to return # endif /* __GNUC__ */ return ""; # endif } #endif /* Output, if appropriate, a usage message for STATE to STREAM. FLAGS are from the set ARGP_HELP_*. */ void __argp_state_help (const struct argp_state *state, FILE *stream, unsigned flags) { if ((!state || ! (state->flags & ARGP_NO_ERRS)) && stream) { if (state && (state->flags & ARGP_LONG_ONLY)) flags |= ARGP_HELP_LONG_ONLY; _help (state ? state->root_argp : 0, state, stream, flags, state ? state->name : __argp_short_program_name ()); if (!state || ! (state->flags & ARGP_NO_EXIT)) { if (flags & ARGP_HELP_EXIT_ERR) exit (argp_err_exit_status); if (flags & ARGP_HELP_EXIT_OK) exit (0); } } } #ifdef weak_alias weak_alias (__argp_state_help, argp_state_help) #endif /* If appropriate, print the printf string FMT and following args, preceded by the program name and ':', to stderr, and followed by a "Try ... --help" message, then exit (1). */ void __argp_error (const struct argp_state *state, const char *fmt, ...) { if (!state || !(state->flags & ARGP_NO_ERRS)) { FILE *stream = state ? state->err_stream : stderr; if (stream) { va_list ap; #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __flockfile (stream); #endif va_start (ap, fmt); #ifdef _LIBC char *buf; if (_IO_vasprintf (&buf, fmt, ap) < 0) buf = NULL; __fxprintf (stream, "%s: %s\n", state ? state->name : __argp_short_program_name (), buf); free (buf); #else fputs_unlocked (state ? state->name : __argp_short_program_name (), stream); putc_unlocked (':', stream); putc_unlocked (' ', stream); vfprintf (stream, fmt, ap); putc_unlocked ('\n', stream); #endif __argp_state_help (state, stream, ARGP_HELP_STD_ERR); va_end (ap); #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif } } } #ifdef weak_alias weak_alias (__argp_error, argp_error) #endif /* Similar to the standard gnu error-reporting function error(), but will respect the ARGP_NO_EXIT and ARGP_NO_ERRS flags in STATE, and will print to STATE->err_stream. This is useful for argument parsing code that is shared between program startup (when exiting is desired) and runtime option parsing (when typically an error code is returned instead). The difference between this function and argp_error is that the latter is for *parsing errors*, and the former is for other problems that occur during parsing but don't reflect a (syntactic) problem with the input. */ void __argp_failure (const struct argp_state *state, int status, int errnum, const char *fmt, ...) { if (!state || !(state->flags & ARGP_NO_ERRS)) { FILE *stream = state ? state->err_stream : stderr; if (stream) { #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __flockfile (stream); #endif #ifdef _LIBC __fxprintf (stream, "%s", state ? state->name : __argp_short_program_name ()); #else fputs_unlocked (state ? state->name : __argp_short_program_name (), stream); #endif if (fmt) { va_list ap; va_start (ap, fmt); #ifdef _LIBC char *buf; if (_IO_vasprintf (&buf, fmt, ap) < 0) buf = NULL; __fxprintf (stream, ": %s", buf); free (buf); #else putc_unlocked (':', stream); putc_unlocked (' ', stream); vfprintf (stream, fmt, ap); #endif va_end (ap); } if (errnum) { char buf[200]; #ifdef _LIBC __fxprintf (stream, ": %s", __strerror_r (errnum, buf, sizeof (buf))); #else char const *s = NULL; putc_unlocked (':', stream); putc_unlocked (' ', stream); # if GNULIB_STRERROR_R_POSIX || HAVE_DECL_STRERROR_R # if !GNULIB_STRERROR_R_POSIX && STRERROR_R_CHAR_P s = __strerror_r (errnum, buf, sizeof buf); # else if (__strerror_r (errnum, buf, sizeof buf) == 0) s = buf; # endif # endif if (! s && ! (s = strerror (errnum))) s = dgettext (state->root_argp->argp_domain, "Unknown system error"); fputs_unlocked (s, stream); #endif } #if _LIBC if (_IO_fwide (stream, 0) > 0) putwc_unlocked (L'\n', stream); else #endif putc_unlocked ('\n', stream); #if _LIBC || (HAVE_FLOCKFILE && HAVE_FUNLOCKFILE) __funlockfile (stream); #endif if (status && (!state || !(state->flags & ARGP_NO_EXIT))) exit (status); } } } #ifdef weak_alias weak_alias (__argp_failure, argp_failure) #endif gnuastro-0.5/bootstrapped/lib/argp-fs-xinl.c0000644000175000017500000000317413217200020016060 00000000000000/* Real definitions for extern inline functions in argp-fmtstream.h Copyright (C) 1997-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #ifdef _LIBC # define ARGP_FS_EI #else # define ARGP_FS_EI _GL_EXTERN_INLINE #endif #undef __OPTIMIZE__ #define __OPTIMIZE__ 1 #include "argp-fmtstream.h" #if 0 /* Not exported. */ /* Add weak aliases. */ #if _LIBC - 0 && !defined (ARGP_FMTSTREAM_USE_LINEWRAP) && defined (weak_alias) weak_alias (__argp_fmtstream_putc, argp_fmtstream_putc) weak_alias (__argp_fmtstream_puts, argp_fmtstream_puts) weak_alias (__argp_fmtstream_write, argp_fmtstream_write) weak_alias (__argp_fmtstream_set_lmargin, argp_fmtstream_set_lmargin) weak_alias (__argp_fmtstream_set_rmargin, argp_fmtstream_set_rmargin) weak_alias (__argp_fmtstream_set_wmargin, argp_fmtstream_set_wmargin) weak_alias (__argp_fmtstream_point, argp_fmtstream_point) #endif #endif gnuastro-0.5/bootstrapped/lib/argp-fmtstream.h0000644000175000017500000002660113217200020016507 00000000000000/* Word-wrapping and line-truncating streams. Copyright (C) 1997-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This package emulates glibc 'line_wrap_stream' semantics for systems that don't have that. If the system does have it, it is just a wrapper for that. This header file is only used internally while compiling argp, and shouldn't be installed. */ #ifndef _ARGP_FMTSTREAM_H #define _ARGP_FMTSTREAM_H #include #include #include /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif #if defined (__GNU_LIBRARY__) && defined (HAVE_LINEWRAP_H) /* line_wrap_stream is available, so use that. */ #define ARGP_FMTSTREAM_USE_LINEWRAP #endif #ifdef ARGP_FMTSTREAM_USE_LINEWRAP /* Just be a simple wrapper for line_wrap_stream; the semantics are *slightly* different, as line_wrap_stream doesn't actually make a new object, it just modifies the given stream (reversibly) to do line-wrapping. Since we control who uses this code, it doesn't matter. */ #include typedef FILE *argp_fmtstream_t; #define argp_make_fmtstream line_wrap_stream #define __argp_make_fmtstream line_wrap_stream #define argp_fmtstream_free line_unwrap_stream #define __argp_fmtstream_free line_unwrap_stream #define __argp_fmtstream_putc(fs,ch) putc(ch,fs) #define argp_fmtstream_putc(fs,ch) putc(ch,fs) #define __argp_fmtstream_puts(fs,str) fputs(str,fs) #define argp_fmtstream_puts(fs,str) fputs(str,fs) #define __argp_fmtstream_write(fs,str,len) fwrite(str,1,len,fs) #define argp_fmtstream_write(fs,str,len) fwrite(str,1,len,fs) #define __argp_fmtstream_printf fprintf #define argp_fmtstream_printf fprintf #define __argp_fmtstream_lmargin line_wrap_lmargin #define argp_fmtstream_lmargin line_wrap_lmargin #define __argp_fmtstream_set_lmargin line_wrap_set_lmargin #define argp_fmtstream_set_lmargin line_wrap_set_lmargin #define __argp_fmtstream_rmargin line_wrap_rmargin #define argp_fmtstream_rmargin line_wrap_rmargin #define __argp_fmtstream_set_rmargin line_wrap_set_rmargin #define argp_fmtstream_set_rmargin line_wrap_set_rmargin #define __argp_fmtstream_wmargin line_wrap_wmargin #define argp_fmtstream_wmargin line_wrap_wmargin #define __argp_fmtstream_set_wmargin line_wrap_set_wmargin #define argp_fmtstream_set_wmargin line_wrap_set_wmargin #define __argp_fmtstream_point line_wrap_point #define argp_fmtstream_point line_wrap_point #else /* !ARGP_FMTSTREAM_USE_LINEWRAP */ /* Guess we have to define our own version. */ struct argp_fmtstream { FILE *stream; /* The stream we're outputting to. */ size_t lmargin, rmargin; /* Left and right margins. */ ssize_t wmargin; /* Margin to wrap to, or -1 to truncate. */ /* Point in buffer to which we've processed for wrapping, but not output. */ size_t point_offs; /* Output column at POINT_OFFS, or -1 meaning 0 but don't add lmargin. */ ssize_t point_col; char *buf; /* Output buffer. */ char *p; /* Current end of text in BUF. */ char *end; /* Absolute end of BUF. */ }; typedef struct argp_fmtstream *argp_fmtstream_t; /* Return an argp_fmtstream that outputs to STREAM, and which prefixes lines written on it with LMARGIN spaces and limits them to RMARGIN columns total. If WMARGIN >= 0, words that extend past RMARGIN are wrapped by replacing the whitespace before them with a newline and WMARGIN spaces. Otherwise, chars beyond RMARGIN are simply dropped until a newline. Returns NULL if there was an error. */ extern argp_fmtstream_t __argp_make_fmtstream (FILE *__stream, size_t __lmargin, size_t __rmargin, ssize_t __wmargin); extern argp_fmtstream_t argp_make_fmtstream (FILE *__stream, size_t __lmargin, size_t __rmargin, ssize_t __wmargin); /* Flush __FS to its stream, and free it (but don't close the stream). */ extern void __argp_fmtstream_free (argp_fmtstream_t __fs); extern void argp_fmtstream_free (argp_fmtstream_t __fs); extern ssize_t __argp_fmtstream_printf (argp_fmtstream_t __fs, const char *__fmt, ...) _GL_ATTRIBUTE_FORMAT ((printf, 2, 3)); extern ssize_t argp_fmtstream_printf (argp_fmtstream_t __fs, const char *__fmt, ...) _GL_ATTRIBUTE_FORMAT ((printf, 2, 3)); #if _LIBC extern int __argp_fmtstream_putc (argp_fmtstream_t __fs, int __ch); extern int argp_fmtstream_putc (argp_fmtstream_t __fs, int __ch); extern int __argp_fmtstream_puts (argp_fmtstream_t __fs, const char *__str); extern int argp_fmtstream_puts (argp_fmtstream_t __fs, const char *__str); extern size_t __argp_fmtstream_write (argp_fmtstream_t __fs, const char *__str, size_t __len); extern size_t argp_fmtstream_write (argp_fmtstream_t __fs, const char *__str, size_t __len); #endif /* Access macros for various bits of state. */ #define argp_fmtstream_lmargin(__fs) ((__fs)->lmargin) #define argp_fmtstream_rmargin(__fs) ((__fs)->rmargin) #define argp_fmtstream_wmargin(__fs) ((__fs)->wmargin) #define __argp_fmtstream_lmargin argp_fmtstream_lmargin #define __argp_fmtstream_rmargin argp_fmtstream_rmargin #define __argp_fmtstream_wmargin argp_fmtstream_wmargin #if _LIBC /* Set __FS's left margin to LMARGIN and return the old value. */ extern size_t argp_fmtstream_set_lmargin (argp_fmtstream_t __fs, size_t __lmargin); extern size_t __argp_fmtstream_set_lmargin (argp_fmtstream_t __fs, size_t __lmargin); /* Set __FS's right margin to __RMARGIN and return the old value. */ extern size_t argp_fmtstream_set_rmargin (argp_fmtstream_t __fs, size_t __rmargin); extern size_t __argp_fmtstream_set_rmargin (argp_fmtstream_t __fs, size_t __rmargin); /* Set __FS's wrap margin to __WMARGIN and return the old value. */ extern size_t argp_fmtstream_set_wmargin (argp_fmtstream_t __fs, size_t __wmargin); extern size_t __argp_fmtstream_set_wmargin (argp_fmtstream_t __fs, size_t __wmargin); /* Return the column number of the current output point in __FS. */ extern size_t argp_fmtstream_point (argp_fmtstream_t __fs); extern size_t __argp_fmtstream_point (argp_fmtstream_t __fs); #endif /* Internal routines. */ extern void _argp_fmtstream_update (argp_fmtstream_t __fs); extern void __argp_fmtstream_update (argp_fmtstream_t __fs); extern int _argp_fmtstream_ensure (argp_fmtstream_t __fs, size_t __amount); extern int __argp_fmtstream_ensure (argp_fmtstream_t __fs, size_t __amount); #if !_LIBC || defined __OPTIMIZE__ /* Inline versions of above routines. */ #if !_LIBC #define __argp_fmtstream_putc argp_fmtstream_putc #define __argp_fmtstream_puts argp_fmtstream_puts #define __argp_fmtstream_write argp_fmtstream_write #define __argp_fmtstream_set_lmargin argp_fmtstream_set_lmargin #define __argp_fmtstream_set_rmargin argp_fmtstream_set_rmargin #define __argp_fmtstream_set_wmargin argp_fmtstream_set_wmargin #define __argp_fmtstream_point argp_fmtstream_point #define __argp_fmtstream_update _argp_fmtstream_update #define __argp_fmtstream_ensure _argp_fmtstream_ensure #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN #ifndef ARGP_FS_EI # define ARGP_FS_EI _GL_INLINE #endif #endif #ifndef ARGP_FS_EI #define ARGP_FS_EI extern inline #endif ARGP_FS_EI size_t __argp_fmtstream_write (argp_fmtstream_t __fs, const char *__str, size_t __len) { if (__fs->p + __len <= __fs->end || __argp_fmtstream_ensure (__fs, __len)) { memcpy (__fs->p, __str, __len); __fs->p += __len; return __len; } else return 0; } ARGP_FS_EI int __argp_fmtstream_puts (argp_fmtstream_t __fs, const char *__str) { size_t __len = strlen (__str); if (__len) { size_t __wrote = __argp_fmtstream_write (__fs, __str, __len); return __wrote == __len ? 0 : -1; } else return 0; } ARGP_FS_EI int __argp_fmtstream_putc (argp_fmtstream_t __fs, int __ch) { if (__fs->p < __fs->end || __argp_fmtstream_ensure (__fs, 1)) return *__fs->p++ = __ch; else return EOF; } /* Set __FS's left margin to __LMARGIN and return the old value. */ ARGP_FS_EI size_t __argp_fmtstream_set_lmargin (argp_fmtstream_t __fs, size_t __lmargin) { size_t __old; if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); __old = __fs->lmargin; __fs->lmargin = __lmargin; return __old; } /* Set __FS's right margin to __RMARGIN and return the old value. */ ARGP_FS_EI size_t __argp_fmtstream_set_rmargin (argp_fmtstream_t __fs, size_t __rmargin) { size_t __old; if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); __old = __fs->rmargin; __fs->rmargin = __rmargin; return __old; } /* Set FS's wrap margin to __WMARGIN and return the old value. */ ARGP_FS_EI size_t __argp_fmtstream_set_wmargin (argp_fmtstream_t __fs, size_t __wmargin) { size_t __old; if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); __old = __fs->wmargin; __fs->wmargin = __wmargin; return __old; } /* Return the column number of the current output point in __FS. */ ARGP_FS_EI size_t __argp_fmtstream_point (argp_fmtstream_t __fs) { if ((size_t) (__fs->p - __fs->buf) > __fs->point_offs) __argp_fmtstream_update (__fs); return __fs->point_col >= 0 ? __fs->point_col : 0; } #if !_LIBC #undef __argp_fmtstream_putc #undef __argp_fmtstream_puts #undef __argp_fmtstream_write #undef __argp_fmtstream_set_lmargin #undef __argp_fmtstream_set_rmargin #undef __argp_fmtstream_set_wmargin #undef __argp_fmtstream_point #undef __argp_fmtstream_update #undef __argp_fmtstream_ensure _GL_INLINE_HEADER_END #endif #endif /* !_LIBC || __OPTIMIZE__ */ #endif /* ARGP_FMTSTREAM_USE_LINEWRAP */ #endif /* argp-fmtstream.h */ gnuastro-0.5/bootstrapped/lib/argp-fmtstream.c0000644000175000017500000003166413217200020016507 00000000000000/* Word-wrapping and line-truncating streams Copyright (C) 1997-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* This package emulates glibc 'line_wrap_stream' semantics for systems that don't have that. */ #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include "argp-fmtstream.h" #include "argp-namefrob.h" #ifndef ARGP_FMTSTREAM_USE_LINEWRAP #ifndef isblank #define isblank(ch) ((ch)==' ' || (ch)=='\t') #endif #ifdef _LIBC # include # include # define __vsnprintf(s, l, f, a) _IO_vsnprintf (s, l, f, a) #endif #define INIT_BUF_SIZE 200 #define PRINTF_SIZE_GUESS 150 /* Return an argp_fmtstream that outputs to STREAM, and which prefixes lines written on it with LMARGIN spaces and limits them to RMARGIN columns total. If WMARGIN >= 0, words that extend past RMARGIN are wrapped by replacing the whitespace before them with a newline and WMARGIN spaces. Otherwise, chars beyond RMARGIN are simply dropped until a newline. Returns NULL if there was an error. */ argp_fmtstream_t __argp_make_fmtstream (FILE *stream, size_t lmargin, size_t rmargin, ssize_t wmargin) { argp_fmtstream_t fs; fs = (struct argp_fmtstream *) malloc (sizeof (struct argp_fmtstream)); if (fs != NULL) { fs->stream = stream; fs->lmargin = lmargin; fs->rmargin = rmargin; fs->wmargin = wmargin; fs->point_col = 0; fs->point_offs = 0; fs->buf = (char *) malloc (INIT_BUF_SIZE); if (! fs->buf) { free (fs); fs = 0; } else { fs->p = fs->buf; fs->end = fs->buf + INIT_BUF_SIZE; } } return fs; } #if 0 /* Not exported. */ #ifdef weak_alias weak_alias (__argp_make_fmtstream, argp_make_fmtstream) #endif #endif /* Flush FS to its stream, and free it (but don't close the stream). */ void __argp_fmtstream_free (argp_fmtstream_t fs) { __argp_fmtstream_update (fs); if (fs->p > fs->buf) { #ifdef _LIBC __fxprintf (fs->stream, "%.*s", (int) (fs->p - fs->buf), fs->buf); #else fwrite_unlocked (fs->buf, 1, fs->p - fs->buf, fs->stream); #endif } free (fs->buf); free (fs); } #if 0 /* Not exported. */ #ifdef weak_alias weak_alias (__argp_fmtstream_free, argp_fmtstream_free) #endif #endif /* Process FS's buffer so that line wrapping is done from POINT_OFFS to the end of its buffer. This code is mostly from glibc stdio/linewrap.c. */ void __argp_fmtstream_update (argp_fmtstream_t fs) { char *buf, *nl; size_t len; /* Scan the buffer for newlines. */ buf = fs->buf + fs->point_offs; while (buf < fs->p) { size_t r; if (fs->point_col == 0 && fs->lmargin != 0) { /* We are starting a new line. Print spaces to the left margin. */ const size_t pad = fs->lmargin; if (fs->p + pad < fs->end) { /* We can fit in them in the buffer by moving the buffer text up and filling in the beginning. */ memmove (buf + pad, buf, fs->p - buf); fs->p += pad; /* Compensate for bigger buffer. */ memset (buf, ' ', pad); /* Fill in the spaces. */ buf += pad; /* Don't bother searching them. */ } else { /* No buffer space for spaces. Must flush. */ size_t i; for (i = 0; i < pad; i++) { #ifdef _LIBC if (_IO_fwide (fs->stream, 0) > 0) putwc_unlocked (L' ', fs->stream); else #endif putc_unlocked (' ', fs->stream); } } fs->point_col = pad; } len = fs->p - buf; nl = memchr (buf, '\n', len); if (fs->point_col < 0) fs->point_col = 0; if (!nl) { /* The buffer ends in a partial line. */ if (fs->point_col + len < fs->rmargin) { /* The remaining buffer text is a partial line and fits within the maximum line width. Advance point for the characters to be written and stop scanning. */ fs->point_col += len; break; } else /* Set the end-of-line pointer for the code below to the end of the buffer. */ nl = fs->p; } else if (fs->point_col + (nl - buf) < (ssize_t) fs->rmargin) { /* The buffer contains a full line that fits within the maximum line width. Reset point and scan the next line. */ fs->point_col = 0; buf = nl + 1; continue; } /* This line is too long. */ r = fs->rmargin - 1; if (fs->wmargin < 0) { /* Truncate the line by overwriting the excess with the newline and anything after it in the buffer. */ if (nl < fs->p) { memmove (buf + (r - fs->point_col), nl, fs->p - nl); fs->p -= buf + (r - fs->point_col) - nl; /* Reset point for the next line and start scanning it. */ fs->point_col = 0; buf += r + 1; /* Skip full line plus \n. */ } else { /* The buffer ends with a partial line that is beyond the maximum line width. Advance point for the characters written, and discard those past the max from the buffer. */ fs->point_col += len; fs->p -= fs->point_col - r; break; } } else { /* Do word wrap. Go to the column just past the maximum line width and scan back for the beginning of the word there. Then insert a line break. */ char *p, *nextline; int i; p = buf + (r + 1 - fs->point_col); while (p >= buf && !isblank ((unsigned char) *p)) --p; nextline = p + 1; /* This will begin the next line. */ if (nextline > buf) { /* Swallow separating blanks. */ if (p >= buf) do --p; while (p >= buf && isblank ((unsigned char) *p)); nl = p + 1; /* The newline will replace the first blank. */ } else { /* A single word that is greater than the maximum line width. Oh well. Put it on an overlong line by itself. */ p = buf + (r + 1 - fs->point_col); /* Find the end of the long word. */ if (p < nl) do ++p; while (p < nl && !isblank ((unsigned char) *p)); if (p == nl) { /* It already ends a line. No fussing required. */ fs->point_col = 0; buf = nl + 1; continue; } /* We will move the newline to replace the first blank. */ nl = p; /* Swallow separating blanks. */ do ++p; while (isblank ((unsigned char) *p)); /* The next line will start here. */ nextline = p; } /* Note: There are a bunch of tests below for NEXTLINE == BUF + LEN + 1; this case is where NL happens to fall at the end of the buffer, and NEXTLINE is in fact empty (and so we need not be careful to maintain its contents). */ if ((nextline == buf + len + 1 ? fs->end - nl < fs->wmargin + 1 : nextline - (nl + 1) < fs->wmargin) && fs->p > nextline) { /* The margin needs more blanks than we removed. */ if (fs->end - fs->p > fs->wmargin + 1) /* Make some space for them. */ { size_t mv = fs->p - nextline; memmove (nl + 1 + fs->wmargin, nextline, mv); nextline = nl + 1 + fs->wmargin; len = nextline + mv - buf; *nl++ = '\n'; } else /* Output the first line so we can use the space. */ { #ifdef _LIBC __fxprintf (fs->stream, "%.*s\n", (int) (nl - fs->buf), fs->buf); #else if (nl > fs->buf) fwrite_unlocked (fs->buf, 1, nl - fs->buf, fs->stream); putc_unlocked ('\n', fs->stream); #endif len += buf - fs->buf; nl = buf = fs->buf; } } else /* We can fit the newline and blanks in before the next word. */ *nl++ = '\n'; if (nextline - nl >= fs->wmargin || (nextline == buf + len + 1 && fs->end - nextline >= fs->wmargin)) /* Add blanks up to the wrap margin column. */ for (i = 0; i < fs->wmargin; ++i) *nl++ = ' '; else for (i = 0; i < fs->wmargin; ++i) #ifdef _LIBC if (_IO_fwide (fs->stream, 0) > 0) putwc_unlocked (L' ', fs->stream); else #endif putc_unlocked (' ', fs->stream); /* Copy the tail of the original buffer into the current buffer position. */ if (nl < nextline) memmove (nl, nextline, buf + len - nextline); len -= nextline - buf; /* Continue the scan on the remaining lines in the buffer. */ buf = nl; /* Restore bufp to include all the remaining text. */ fs->p = nl + len; /* Reset the counter of what has been output this line. If wmargin is 0, we want to avoid the lmargin getting added, so we set point_col to a magic value of -1 in that case. */ fs->point_col = fs->wmargin ? fs->wmargin : -1; } } /* Remember that we've scanned as far as the end of the buffer. */ fs->point_offs = fs->p - fs->buf; } /* Ensure that FS has space for AMOUNT more bytes in its buffer, either by growing the buffer, or by flushing it. True is returned iff we succeed. */ int __argp_fmtstream_ensure (struct argp_fmtstream *fs, size_t amount) { if ((size_t) (fs->end - fs->p) < amount) { ssize_t wrote; /* Flush FS's buffer. */ __argp_fmtstream_update (fs); #ifdef _LIBC __fxprintf (fs->stream, "%.*s", (int) (fs->p - fs->buf), fs->buf); wrote = fs->p - fs->buf; #else wrote = fwrite_unlocked (fs->buf, 1, fs->p - fs->buf, fs->stream); #endif if (wrote == fs->p - fs->buf) { fs->p = fs->buf; fs->point_offs = 0; } else { fs->p -= wrote; fs->point_offs -= wrote; memmove (fs->buf, fs->buf + wrote, fs->p - fs->buf); return 0; } if ((size_t) (fs->end - fs->buf) < amount) /* Gotta grow the buffer. */ { size_t old_size = fs->end - fs->buf; size_t new_size = old_size + amount; char *new_buf; if (new_size < old_size || ! (new_buf = realloc (fs->buf, new_size))) { __set_errno (ENOMEM); return 0; } fs->buf = new_buf; fs->end = new_buf + new_size; fs->p = fs->buf; } } return 1; } ssize_t __argp_fmtstream_printf (struct argp_fmtstream *fs, const char *fmt, ...) { int out; size_t avail; size_t size_guess = PRINTF_SIZE_GUESS; /* How much space to reserve. */ do { va_list args; if (! __argp_fmtstream_ensure (fs, size_guess)) return -1; va_start (args, fmt); avail = fs->end - fs->p; out = __vsnprintf (fs->p, avail, fmt, args); va_end (args); if ((size_t) out >= avail) size_guess = out + 1; } while ((size_t) out >= avail); fs->p += out; return out; } #if 0 /* Not exported. */ #ifdef weak_alias weak_alias (__argp_fmtstream_printf, argp_fmtstream_printf) #endif #endif #endif /* !ARGP_FMTSTREAM_USE_LINEWRAP */ gnuastro-0.5/bootstrapped/lib/argp-eexst.c0000644000175000017500000000220713217200020015624 00000000000000/* Default definition for ARGP_ERR_EXIT_STATUS Copyright (C) 1997, 2009-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifdef HAVE_CONFIG_H # include #endif #include #include "argp.h" /* The exit status that argp will use when exiting due to a parsing error. If not defined or set by the user program, this defaults to EX_USAGE from . */ error_t argp_err_exit_status = EX_USAGE; gnuastro-0.5/bootstrapped/lib/argp-ba.c0000644000175000017500000000305713217200020015062 00000000000000/* Default definition for ARGP_PROGRAM_BUG_ADDRESS. Copyright (C) 1996-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ /* If set by the user program, it should point to string that is the bug-reporting address for the program. It will be printed by argp_help if the ARGP_HELP_BUG_ADDR flag is set (as it is by various standard help messages), embedded in a sentence that says something like "Report bugs to ADDR." */ const char *argp_program_bug_address /* This variable should be zero-initialized. On most systems, putting it into BSS is sufficient. Not so on Mac OS X 10.3 and 10.4, see . */ #if defined __ELF__ /* On ELF systems, variables in BSS behave well. */ #else = (const char *) 0 #endif ; gnuastro-0.5/bootstrapped/lib/argp.h0000644000175000017500000007143413217200050014516 00000000000000/* Hierarchical argument parsing, layered over getopt. Copyright (C) 1995-2017 Free Software Foundation, Inc. This file is part of the GNU C Library. Written by Miles Bader . This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #ifndef _ARGP_H #define _ARGP_H #include #include #include #include #define __need_error_t #include #ifndef __THROW # define __THROW #endif #ifndef __NTH # define __NTH(fct) fct __THROW #endif /* The __attribute__ feature is available in gcc versions 2.5 and later. The __-protected variants of the attributes 'format' and 'printf' are accepted by gcc versions 2.6.4 (effectively 2.7) and later. We enable _GL_ATTRIBUTE_FORMAT only if these are supported too, because gnulib and libintl do '#define printf __printf__' when they override the 'printf' function. */ #if __GNUC__ > 2 || (__GNUC__ == 2 && __GNUC_MINOR__ >= 7) # define _GL_ATTRIBUTE_FORMAT(spec) __attribute__ ((__format__ spec)) #else # define _GL_ATTRIBUTE_FORMAT(spec) /* empty */ #endif /* GCC 2.95 and later have "__restrict"; C99 compilers have "restrict", and "configure" may have defined "restrict". Other compilers use __restrict, __restrict__, and _Restrict, and 'configure' might #define 'restrict' to those words. */ #ifndef __restrict # if ! (2 < __GNUC__ || (2 == __GNUC__ && 95 <= __GNUC_MINOR__)) # if 199901L <= __STDC_VERSION__ # define __restrict restrict # else # define __restrict # endif # endif #endif #ifndef __error_t_defined typedef int error_t; # define __error_t_defined #endif #ifdef __cplusplus extern "C" { #endif /* A description of a particular option. A pointer to an array of these is passed in the OPTIONS field of an argp structure. Each option entry can correspond to one long option and/or one short option; more names for the same option can be added by following an entry in an option array with options having the OPTION_ALIAS flag set. */ struct argp_option { /* The long option name. For more than one name for the same option, you can use following options with the OPTION_ALIAS flag set. */ const char *name; /* What key is returned for this option. If > 0 and printable, then it's also accepted as a short option. */ int key; /* If non-NULL, this is the name of the argument associated with this option, which is required unless the OPTION_ARG_OPTIONAL flag is set. */ const char *arg; /* OPTION_ flags. */ int flags; /* The doc string for this option. If both NAME and KEY are 0, This string will be printed outdented from the normal option column, making it useful as a group header (it will be the first thing printed in its group); in this usage, it's conventional to end the string with a ':'. Write the initial value as N_("TEXT") if you want xgettext to collect it into a POT file. */ const char *doc; /* The group this option is in. In a long help message, options are sorted alphabetically within each group, and the groups presented in the order 0, 1, 2, ..., n, -m, ..., -2, -1. Every entry in an options array with if this field 0 will inherit the group number of the previous entry, or zero if it's the first one, unless its a group header (NAME and KEY both 0), in which case, the previous entry + 1 is the default. Automagic options such as --help are put into group -1. */ int group; /* Pointer to value. IMPORTANT: A Gnuastro addition. */ void *value; /* Type of value (see lib/gnuastro/data.h). IMPORTANT: A Gnuastro addition. */ int type; /* Acceptable range of value (see lib/options.h). IMPORTANT: A Gnuastro addition. */ int range; /* Is this option mandatory? (see lib/options.h). IMPORTANT: A Gnuastro addition. */ unsigned char mandatory; /* Is value already set or not? (see lib/options.h). IMPORTANT: A Gnuastro addition. */ unsigned char set; /* Function to process the given value. Arguments to the function: struct argp_option *option: This argp_option. char *arg: String given by the user. char *filename: Filename option was read from. size_t lineno: Line number of option in file. void *struct: Pointer to main program struct. IMPORTANT: A Gnuastro addition. */ void *(*func)(struct argp_option *, char *, char *, size_t, void *); }; /* The argument associated with this option is optional. */ #define OPTION_ARG_OPTIONAL 0x1 /* This option isn't displayed in any help messages. */ #define OPTION_HIDDEN 0x2 /* This option is an alias for the closest previous non-alias option. This means that it will be displayed in the same help entry, and will inherit fields other than NAME and KEY from the aliased option. */ #define OPTION_ALIAS 0x4 /* This option isn't actually an option (and so should be ignored by the actual option parser), but rather an arbitrary piece of documentation that should be displayed in much the same manner as the options. If this flag is set, then the option NAME field is displayed unmodified (e.g., no '--' prefix is added) at the left-margin (where a *short* option would normally be displayed), and the documentation string in the normal place. The NAME field will be translated using gettext, unless OPTION_NO_TRANS is set (see below). For purposes of sorting, any leading whitespace and punctuation is ignored, except that if the first non-whitespace character is not '-', this entry is displayed after all options (and OPTION_DOC entries with a leading '-') in the same group. */ #define OPTION_DOC 0x8 /* This option shouldn't be included in "long" usage messages (but is still included in help messages). This is mainly intended for options that are completely documented in an argp's ARGS_DOC field, in which case including the option in the generic usage list would be redundant. For instance, if ARGS_DOC is "FOO BAR\n-x BLAH", and the '-x' option's purpose is to distinguish these two cases, -x should probably be marked OPTION_NO_USAGE. */ #define OPTION_NO_USAGE 0x10 /* Valid only in conjunction with OPTION_DOC. This option disables translation of option name. */ #define OPTION_NO_TRANS 0x20 struct argp; /* fwd declare this type */ struct argp_state; /* " */ struct argp_child; /* " */ /* The type of a pointer to an argp parsing function. */ typedef error_t (*argp_parser_t) (int __key, char *__arg, struct argp_state *__state); /* What to return for unrecognized keys. For special ARGP_KEY_ keys, such returns will simply be ignored. For user keys, this error will be turned into EINVAL (if the call to argp_parse is such that errors are propagated back to the user instead of exiting); returning EINVAL itself would result in an immediate stop to parsing in *all* cases. */ #define ARGP_ERR_UNKNOWN E2BIG /* Hurd should never need E2BIG. XXX */ /* Special values for the KEY argument to an argument parsing function. ARGP_ERR_UNKNOWN should be returned if they aren't understood. The sequence of keys to a parsing function is either (where each uppercased word should be prefixed by 'ARGP_KEY_' and opt is a user key): INIT opt... NO_ARGS END SUCCESS -- No non-option arguments at all or INIT (opt | ARG)... END SUCCESS -- All non-option args parsed or INIT (opt | ARG)... SUCCESS -- Some non-option arg unrecognized The third case is where every parser returned ARGP_KEY_UNKNOWN for an argument, in which case parsing stops at that argument (returning the unparsed arguments to the caller of argp_parse if requested, or stopping with an error message if not). If an error occurs (either detected by argp, or because the parsing function returned an error value), then the parser is called with ARGP_KEY_ERROR, and no further calls are made. */ /* This is not an option at all, but rather a command line argument. If a parser receiving this key returns success, the fact is recorded, and the ARGP_KEY_NO_ARGS case won't be used. HOWEVER, if while processing the argument, a parser function decrements the NEXT field of the state it's passed, the option won't be considered processed; this is to allow you to actually modify the argument (perhaps into an option), and have it processed again. */ #define ARGP_KEY_ARG 0 /* There are remaining arguments not parsed by any parser, which may be found starting at (STATE->argv + STATE->next). If success is returned, but STATE->next left untouched, it's assumed that all arguments were consume, otherwise, the parser should adjust STATE->next to reflect any arguments consumed. */ #define ARGP_KEY_ARGS 0x1000006 /* There are no more command line arguments at all. */ #define ARGP_KEY_END 0x1000001 /* Because it's common to want to do some special processing if there aren't any non-option args, user parsers are called with this key if they didn't successfully process any non-option arguments. Called just before ARGP_KEY_END (where more general validity checks on previously parsed arguments can take place). */ #define ARGP_KEY_NO_ARGS 0x1000002 /* Passed in before any parsing is done. Afterwards, the values of each element of the CHILD_INPUT field, if any, in the state structure is copied to each child's state to be the initial value of the INPUT field. */ #define ARGP_KEY_INIT 0x1000003 /* Use after all other keys, including SUCCESS & END. */ #define ARGP_KEY_FINI 0x1000007 /* Passed in when parsing has successfully been completed (even if there are still arguments remaining). */ #define ARGP_KEY_SUCCESS 0x1000004 /* Passed in if an error occurs. */ #define ARGP_KEY_ERROR 0x1000005 /* An argp structure contains a set of options declarations, a function to deal with parsing one, documentation string, a possible vector of child argp's, and perhaps a function to filter help output. When actually parsing options, getopt is called with the union of all the argp structures chained together through their CHILD pointers, with conflicts being resolved in favor of the first occurrence in the chain. */ struct argp { /* An array of argp_option structures, terminated by an entry with both NAME and KEY having a value of 0. */ const struct argp_option *options; /* What to do with an option from this structure. KEY is the key associated with the option, and ARG is any associated argument (NULL if none was supplied). If KEY isn't understood, ARGP_ERR_UNKNOWN should be returned. If a non-zero, non-ARGP_ERR_UNKNOWN value is returned, then parsing is stopped immediately, and that value is returned from argp_parse(). For special (non-user-supplied) values of KEY, see the ARGP_KEY_ definitions below. */ argp_parser_t parser; /* A string describing what other arguments are wanted by this program. It is only used by argp_usage to print the "Usage:" message. If it contains newlines, the strings separated by them are considered alternative usage patterns, and printed on separate lines (lines after the first are prefix by " or: " instead of "Usage:"). */ const char *args_doc; /* If non-NULL, a string containing extra text to be printed before and after the options in a long help message (separated by a vertical tab '\v' character). Write the initial value as N_("BEFORE-TEXT") "\v" N_("AFTER-TEXT") if you want xgettext to collect the two pieces of text into a POT file. */ const char *doc; /* A vector of argp_children structures, terminated by a member with a 0 argp field, pointing to child argps should be parsed with this one. Any conflicts are resolved in favor of this argp, or early argps in the CHILDREN list. This field is useful if you use libraries that supply their own argp structure, which you want to use in conjunction with your own. */ const struct argp_child *children; /* If non-zero, this should be a function to filter the output of help messages. KEY is either a key from an option, in which case TEXT is that option's help text, or a special key from the ARGP_KEY_HELP_ defines, below, describing which other help text TEXT is. The function should return either TEXT, if it should be used as-is, a replacement string, which should be malloced, and will be freed by argp, or NULL, meaning "print nothing". The value for TEXT is *after* any translation has been done, so if any of the replacement text also needs translation, that should be done by the filter function. INPUT is either the input supplied to argp_parse, or NULL, if argp_help was called directly. */ char *(*help_filter) (int __key, const char *__text, void *__input); /* If non-zero the strings used in the argp library are translated using the domain described by this string. Otherwise the currently installed default domain is used. */ const char *argp_domain; }; /* Possible KEY arguments to a help filter function. */ #define ARGP_KEY_HELP_PRE_DOC 0x2000001 /* Help text preceding options. */ #define ARGP_KEY_HELP_POST_DOC 0x2000002 /* Help text following options. */ #define ARGP_KEY_HELP_HEADER 0x2000003 /* Option header string. */ #define ARGP_KEY_HELP_EXTRA 0x2000004 /* After all other documentation; TEXT is NULL for this key. */ /* Explanatory note emitted when duplicate option arguments have been suppressed. */ #define ARGP_KEY_HELP_DUP_ARGS_NOTE 0x2000005 #define ARGP_KEY_HELP_ARGS_DOC 0x2000006 /* Argument doc string. */ /* When an argp has a non-zero CHILDREN field, it should point to a vector of argp_child structures, each of which describes a subsidiary argp. */ struct argp_child { /* The child parser. */ const struct argp *argp; /* Flags for this child. */ int flags; /* If non-zero, an optional header to be printed in help output before the child options. As a side-effect, a non-zero value forces the child options to be grouped together; to achieve this effect without actually printing a header string, use a value of "". */ const char *header; /* Where to group the child options relative to the other ("consolidated") options in the parent argp; the values are the same as the GROUP field in argp_option structs, but all child-groupings follow parent options at a particular group level. If both this field and HEADER are zero, then they aren't grouped at all, but rather merged with the parent options (merging the child's grouping levels with the parents). */ int group; }; /* Parsing state. This is provided to parsing functions called by argp, which may examine and, as noted, modify fields. */ struct argp_state { /* The top level ARGP being parsed. */ const struct argp *root_argp; /* The argument vector being parsed. May be modified. */ int argc; char **argv; /* The index in ARGV of the next arg that to be parsed. May be modified. */ int next; /* The flags supplied to argp_parse. May be modified. */ unsigned flags; /* While calling a parsing function with a key of ARGP_KEY_ARG, this is the number of the current arg, starting at zero, and incremented after each such call returns. At all other times, this is the number of such arguments that have been processed. */ unsigned arg_num; /* If non-zero, the index in ARGV of the first argument following a special '--' argument (which prevents anything following being interpreted as an option). Only set once argument parsing has proceeded past this point. */ int quoted; /* An arbitrary pointer passed in from the user. */ void *input; /* Values to pass to child parsers. This vector will be the same length as the number of children for the current parser. */ void **child_inputs; /* For the parser's use. Initialized to 0. */ void *hook; /* The name used when printing messages. This is initialized to ARGV[0], or PROGRAM_INVOCATION_NAME if that is unavailable. */ char *name; /* Streams used when argp prints something. */ FILE *err_stream; /* For errors; initialized to stderr. */ FILE *out_stream; /* For information; initialized to stdout. */ void *pstate; /* Private, for use by argp. */ }; /* Flags for argp_parse (note that the defaults are those that are convenient for program command line parsing): */ /* Don't ignore the first element of ARGV. Normally (and always unless ARGP_NO_ERRS is set) the first element of the argument vector is skipped for option parsing purposes, as it corresponds to the program name in a command line. */ #define ARGP_PARSE_ARGV0 0x01 /* Don't print error messages for unknown options to stderr; unless this flag is set, ARGP_PARSE_ARGV0 is ignored, as ARGV[0] is used as the program name in the error messages. This flag implies ARGP_NO_EXIT (on the assumption that silent exiting upon errors is bad behaviour). */ #define ARGP_NO_ERRS 0x02 /* Don't parse any non-option args. Normally non-option args are parsed by calling the parse functions with a key of ARGP_KEY_ARG, and the actual arg as the value. Since it's impossible to know which parse function wants to handle it, each one is called in turn, until one returns 0 or an error other than ARGP_ERR_UNKNOWN; if an argument is handled by no one, the argp_parse returns prematurely (but with a return value of 0). If all args have been parsed without error, all parsing functions are called one last time with a key of ARGP_KEY_END. This flag needn't normally be set, as the normal behavior is to stop parsing as soon as some argument can't be handled. */ #define ARGP_NO_ARGS 0x04 /* Parse options and arguments in the same order they occur on the command line -- normally they're rearranged so that all options come first. */ #define ARGP_IN_ORDER 0x08 /* Don't provide the standard long option --help, which causes usage and option help information to be output to stdout, and exit (0) called. */ #define ARGP_NO_HELP 0x10 /* Don't exit on errors (they may still result in error messages). */ #define ARGP_NO_EXIT 0x20 /* Use the gnu getopt "long-only" rules for parsing arguments. */ #define ARGP_LONG_ONLY 0x40 /* Turns off any message-printing/exiting options. */ #define ARGP_SILENT (ARGP_NO_EXIT | ARGP_NO_ERRS | ARGP_NO_HELP) /* Parse the options strings in ARGC & ARGV according to the options in ARGP. FLAGS is one of the ARGP_ flags above. If ARG_INDEX is non-NULL, the index in ARGV of the first unparsed option is returned in it. If an unknown option is present, ARGP_ERR_UNKNOWN is returned; if some parser routine returned a non-zero value, it is returned; otherwise 0 is returned. This function may also call exit unless the ARGP_NO_HELP flag is set. INPUT is a pointer to a value to be passed in to the parser. */ extern error_t argp_parse (const struct argp *__restrict __argp, int /*argc*/, char **__restrict /*argv*/, unsigned __flags, int *__restrict __arg_index, void *__restrict __input); extern error_t __argp_parse (const struct argp *__restrict __argp, int /*argc*/, char **__restrict /*argv*/, unsigned __flags, int *__restrict __arg_index, void *__restrict __input); /* Global variables. */ /* GNULIB makes sure both program_invocation_name and program_invocation_short_name are available */ #ifdef GNULIB_PROGRAM_INVOCATION_NAME extern char *program_invocation_name; # undef HAVE_DECL_PROGRAM_INVOCATION_NAME # define HAVE_DECL_PROGRAM_INVOCATION_NAME 1 #endif #ifdef GNULIB_PROGRAM_INVOCATION_SHORT_NAME extern char *program_invocation_short_name; # undef HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME # define HAVE_DECL_PROGRAM_INVOCATION_SHORT_NAME 1 #endif /* If defined or set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which will print this string followed by a newline and exit (unless the ARGP_NO_EXIT flag is used). Overridden by ARGP_PROGRAM_VERSION_HOOK. */ extern const char *argp_program_version; /* If defined or set by the user program to a non-zero value, then a default option --version is added (unless the ARGP_NO_HELP flag is used), which calls this function with a stream to print the version to and a pointer to the current parsing state, and then exits (unless the ARGP_NO_EXIT flag is used). This variable takes precedent over ARGP_PROGRAM_VERSION. */ extern void (*argp_program_version_hook) (FILE *__restrict __stream, struct argp_state *__restrict __state); /* If defined or set by the user program, it should point to string that is the bug-reporting address for the program. It will be printed by argp_help if the ARGP_HELP_BUG_ADDR flag is set (as it is by various standard help messages), embedded in a sentence that says something like "Report bugs to ADDR." */ extern const char *argp_program_bug_address; /* The exit status that argp will use when exiting due to a parsing error. If not defined or set by the user program, this defaults to EX_USAGE from . */ extern error_t argp_err_exit_status; /* Flags for argp_help. */ #define ARGP_HELP_USAGE 0x01 /* a Usage: message. */ #define ARGP_HELP_SHORT_USAGE 0x02 /* " but don't actually print options. */ #define ARGP_HELP_SEE 0x04 /* a "Try ... for more help" message. */ #define ARGP_HELP_LONG 0x08 /* a long help message. */ #define ARGP_HELP_PRE_DOC 0x10 /* doc string preceding long help. */ #define ARGP_HELP_POST_DOC 0x20 /* doc string following long help. */ #define ARGP_HELP_DOC (ARGP_HELP_PRE_DOC | ARGP_HELP_POST_DOC) #define ARGP_HELP_BUG_ADDR 0x40 /* bug report address */ #define ARGP_HELP_LONG_ONLY 0x80 /* modify output appropriately to reflect ARGP_LONG_ONLY mode. */ /* These ARGP_HELP flags are only understood by argp_state_help. */ #define ARGP_HELP_EXIT_ERR 0x100 /* Call exit(1) instead of returning. */ #define ARGP_HELP_EXIT_OK 0x200 /* Call exit(0) instead of returning. */ /* The standard thing to do after a program command line parsing error, if an error message has already been printed. */ #define ARGP_HELP_STD_ERR \ (ARGP_HELP_SEE | ARGP_HELP_EXIT_ERR) /* The standard thing to do after a program command line parsing error, if no more specific error message has been printed. */ #define ARGP_HELP_STD_USAGE \ (ARGP_HELP_SHORT_USAGE | ARGP_HELP_SEE | ARGP_HELP_EXIT_ERR) /* The standard thing to do in response to a --help option. */ #define ARGP_HELP_STD_HELP \ (ARGP_HELP_SHORT_USAGE | ARGP_HELP_LONG | ARGP_HELP_EXIT_OK \ | ARGP_HELP_DOC | ARGP_HELP_BUG_ADDR) /* Output a usage message for ARGP to STREAM. FLAGS are from the set ARGP_HELP_*. */ extern void argp_help (const struct argp *__restrict __argp, FILE *__restrict __stream, unsigned __flags, char *__restrict __name); extern void __argp_help (const struct argp *__restrict __argp, FILE *__restrict __stream, unsigned __flags, char *__name); /* The following routines are intended to be called from within an argp parsing routine (thus taking an argp_state structure as the first argument). They may or may not print an error message and exit, depending on the flags in STATE -- in any case, the caller should be prepared for them *not* to exit, and should return an appropriate error after calling them. [argp_usage & argp_error should probably be called argp_state_..., but they're used often enough that they should be short] */ /* Output, if appropriate, a usage message for STATE to STREAM. FLAGS are from the set ARGP_HELP_*. */ extern void argp_state_help (const struct argp_state *__restrict __state, FILE *__restrict __stream, unsigned int __flags); extern void __argp_state_help (const struct argp_state *__restrict __state, FILE *__restrict __stream, unsigned int __flags); #if _LIBC /* Possibly output the standard usage message for ARGP to stderr and exit. */ extern void argp_usage (const struct argp_state *__state); extern void __argp_usage (const struct argp_state *__state); #endif /* If appropriate, print the printf string FMT and following args, preceded by the program name and ':', to stderr, and followed by a "Try ... --help" message, then exit (1). */ extern void argp_error (const struct argp_state *__restrict __state, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 2, 3)); extern void __argp_error (const struct argp_state *__restrict __state, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 2, 3)); /* Similar to the standard gnu error-reporting function error(), but will respect the ARGP_NO_EXIT and ARGP_NO_ERRS flags in STATE, and will print to STATE->err_stream. This is useful for argument parsing code that is shared between program startup (when exiting is desired) and runtime option parsing (when typically an error code is returned instead). The difference between this function and argp_error is that the latter is for *parsing errors*, and the former is for other problems that occur during parsing but don't reflect a (syntactic) problem with the input. */ extern void argp_failure (const struct argp_state *__restrict __state, int __status, int __errnum, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 4, 5)); extern void __argp_failure (const struct argp_state *__restrict __state, int __status, int __errnum, const char *__restrict __fmt, ...) _GL_ATTRIBUTE_FORMAT ((__printf__, 4, 5)); #if _LIBC /* Returns true if the option OPT is a valid short option. */ extern int _option_is_short (const struct argp_option *__opt) __THROW; extern int __option_is_short (const struct argp_option *__opt) __THROW; /* Returns true if the option OPT is in fact the last (unused) entry in an options array. */ extern int _option_is_end (const struct argp_option *__opt) __THROW; extern int __option_is_end (const struct argp_option *__opt) __THROW; #endif /* Return the input field for ARGP in the parser corresponding to STATE; used by the help routines. */ extern void *_argp_input (const struct argp *__restrict __argp, const struct argp_state *__restrict __state) __THROW; extern void *__argp_input (const struct argp *__restrict __argp, const struct argp_state *__restrict __state) __THROW; #if !_LIBC || defined __USE_EXTERN_INLINES # if !_LIBC # define __argp_usage argp_usage # define __argp_state_help argp_state_help # define __option_is_short _option_is_short # define __option_is_end _option_is_end #ifndef _GL_INLINE_HEADER_BEGIN #error "Please include config.h first." #endif _GL_INLINE_HEADER_BEGIN # ifndef ARGP_EI # define ARGP_EI _GL_INLINE # endif # endif # ifndef ARGP_EI # define ARGP_EI __extern_inline # endif ARGP_EI void __argp_usage (const struct argp_state *__state) { __argp_state_help (__state, stderr, ARGP_HELP_STD_USAGE); } ARGP_EI int __NTH (__option_is_short (const struct argp_option *__opt)) { if (__opt->flags & OPTION_DOC) return 0; else { int __key = __opt->key; return __key > 0 && __key <= UCHAR_MAX && isprint (__key); } } ARGP_EI int __NTH (__option_is_end (const struct argp_option *__opt)) { return !__opt->key && !__opt->name && !__opt->doc && !__opt->group; } # if !_LIBC # undef __argp_usage # undef __argp_state_help # undef __option_is_short # undef __option_is_end _GL_INLINE_HEADER_END # endif #endif /* Use extern inlines. */ #ifdef __cplusplus } #endif #endif /* argp.h */ gnuastro-0.5/bootstrapped/lib/alloca.c0000644000175000017500000003445413217200020015011 00000000000000/* alloca.c -- allocate automatically reclaimed memory (Mostly) portable public-domain implementation -- D A Gwyn This implementation of the PWB library alloca function, which is used to allocate space off the run-time stack so that it is automatically reclaimed upon procedure exit, was inspired by discussions with J. Q. Johnson of Cornell. J.Otto Tennant contributed the Cray support. There are some preprocessor constants that can be defined when compiling for your specific system, for improved efficiency; however, the defaults should be okay. The general concept of this implementation is to keep track of all alloca-allocated blocks, and reclaim any that are found to be deeper in the stack than the current invocation. This heuristic does not reclaim storage as soon as it becomes invalid, but it will do so eventually. As a special case, alloca(0) reclaims storage without allocating any. It is a good idea to use alloca(0) in your main control loop, etc. to force garbage collection. */ #include #include #include #include #ifdef emacs # include "lisp.h" # include "blockinput.h" # ifdef EMACS_FREE # undef free # define free EMACS_FREE # endif #else # define memory_full() abort () #endif /* If compiling with GCC 2, this file's not needed. */ #if !defined (__GNUC__) || __GNUC__ < 2 /* If someone has defined alloca as a macro, there must be some other way alloca is supposed to work. */ # ifndef alloca # ifdef emacs # ifdef static /* actually, only want this if static is defined as "" -- this is for usg, in which emacs must undefine static in order to make unexec workable */ # ifndef STACK_DIRECTION you lose -- must know STACK_DIRECTION at compile-time /* Using #error here is not wise since this file should work for old and obscure compilers. */ # endif /* STACK_DIRECTION undefined */ # endif /* static */ # endif /* emacs */ /* If your stack is a linked list of frames, you have to provide an "address metric" ADDRESS_FUNCTION macro. */ # if defined (CRAY) && defined (CRAY_STACKSEG_END) long i00afunc (); # define ADDRESS_FUNCTION(arg) (char *) i00afunc (&(arg)) # else # define ADDRESS_FUNCTION(arg) &(arg) # endif /* Define STACK_DIRECTION if you know the direction of stack growth for your system; otherwise it will be automatically deduced at run-time. STACK_DIRECTION > 0 => grows toward higher addresses STACK_DIRECTION < 0 => grows toward lower addresses STACK_DIRECTION = 0 => direction of growth unknown */ # ifndef STACK_DIRECTION # define STACK_DIRECTION 0 /* Direction unknown. */ # endif # if STACK_DIRECTION != 0 # define STACK_DIR STACK_DIRECTION /* Known at compile-time. */ # else /* STACK_DIRECTION == 0; need run-time code. */ static int stack_dir; /* 1 or -1 once known. */ # define STACK_DIR stack_dir static int find_stack_direction (int *addr, int depth) { int dir, dummy = 0; if (! addr) addr = &dummy; *addr = addr < &dummy ? 1 : addr == &dummy ? 0 : -1; dir = depth ? find_stack_direction (addr, depth - 1) : 0; return dir + dummy; } # endif /* STACK_DIRECTION == 0 */ /* An "alloca header" is used to: (a) chain together all alloca'ed blocks; (b) keep track of stack depth. It is very important that sizeof(header) agree with malloc alignment chunk size. The following default should work okay. */ # ifndef ALIGN_SIZE # define ALIGN_SIZE sizeof(double) # endif typedef union hdr { char align[ALIGN_SIZE]; /* To force sizeof(header). */ struct { union hdr *next; /* For chaining headers. */ char *deep; /* For stack depth measure. */ } h; } header; static header *last_alloca_header = NULL; /* -> last alloca header. */ /* Return a pointer to at least SIZE bytes of storage, which will be automatically reclaimed upon exit from the procedure that called alloca. Originally, this space was supposed to be taken from the current stack frame of the caller, but that method cannot be made to work for some implementations of C, for example under Gould's UTX/32. */ void * alloca (size_t size) { auto char probe; /* Probes stack depth: */ register char *depth = ADDRESS_FUNCTION (probe); # if STACK_DIRECTION == 0 if (STACK_DIR == 0) /* Unknown growth direction. */ STACK_DIR = find_stack_direction (NULL, (size & 1) + 20); # endif /* Reclaim garbage, defined as all alloca'd storage that was allocated from deeper in the stack than currently. */ { register header *hp; /* Traverses linked list. */ # ifdef emacs BLOCK_INPUT; # endif for (hp = last_alloca_header; hp != NULL;) if ((STACK_DIR > 0 && hp->h.deep > depth) || (STACK_DIR < 0 && hp->h.deep < depth)) { register header *np = hp->h.next; free (hp); /* Collect garbage. */ hp = np; /* -> next header. */ } else break; /* Rest are not deeper. */ last_alloca_header = hp; /* -> last valid storage. */ # ifdef emacs UNBLOCK_INPUT; # endif } if (size == 0) return NULL; /* No allocation required. */ /* Allocate combined header + user data storage. */ { /* Address of header. */ register header *new; size_t combined_size = sizeof (header) + size; if (combined_size < sizeof (header)) memory_full (); new = malloc (combined_size); if (! new) memory_full (); new->h.next = last_alloca_header; new->h.deep = depth; last_alloca_header = new; /* User storage begins just after header. */ return (void *) (new + 1); } } # if defined (CRAY) && defined (CRAY_STACKSEG_END) # ifdef DEBUG_I00AFUNC # include # endif # ifndef CRAY_STACK # define CRAY_STACK # ifndef CRAY2 /* Stack structures for CRAY-1, CRAY X-MP, and CRAY Y-MP */ struct stack_control_header { long shgrow:32; /* Number of times stack has grown. */ long shaseg:32; /* Size of increments to stack. */ long shhwm:32; /* High water mark of stack. */ long shsize:32; /* Current size of stack (all segments). */ }; /* The stack segment linkage control information occurs at the high-address end of a stack segment. (The stack grows from low addresses to high addresses.) The initial part of the stack segment linkage control information is 0200 (octal) words. This provides for register storage for the routine which overflows the stack. */ struct stack_segment_linkage { long ss[0200]; /* 0200 overflow words. */ long sssize:32; /* Number of words in this segment. */ long ssbase:32; /* Offset to stack base. */ long:32; long sspseg:32; /* Offset to linkage control of previous segment of stack. */ long:32; long sstcpt:32; /* Pointer to task common address block. */ long sscsnm; /* Private control structure number for microtasking. */ long ssusr1; /* Reserved for user. */ long ssusr2; /* Reserved for user. */ long sstpid; /* Process ID for pid based multi-tasking. */ long ssgvup; /* Pointer to multitasking thread giveup. */ long sscray[7]; /* Reserved for Cray Research. */ long ssa0; long ssa1; long ssa2; long ssa3; long ssa4; long ssa5; long ssa6; long ssa7; long sss0; long sss1; long sss2; long sss3; long sss4; long sss5; long sss6; long sss7; }; # else /* CRAY2 */ /* The following structure defines the vector of words returned by the STKSTAT library routine. */ struct stk_stat { long now; /* Current total stack size. */ long maxc; /* Amount of contiguous space which would be required to satisfy the maximum stack demand to date. */ long high_water; /* Stack high-water mark. */ long overflows; /* Number of stack overflow ($STKOFEN) calls. */ long hits; /* Number of internal buffer hits. */ long extends; /* Number of block extensions. */ long stko_mallocs; /* Block allocations by $STKOFEN. */ long underflows; /* Number of stack underflow calls ($STKRETN). */ long stko_free; /* Number of deallocations by $STKRETN. */ long stkm_free; /* Number of deallocations by $STKMRET. */ long segments; /* Current number of stack segments. */ long maxs; /* Maximum number of stack segments so far. */ long pad_size; /* Stack pad size. */ long current_address; /* Current stack segment address. */ long current_size; /* Current stack segment size. This number is actually corrupted by STKSTAT to include the fifteen word trailer area. */ long initial_address; /* Address of initial segment. */ long initial_size; /* Size of initial segment. */ }; /* The following structure describes the data structure which trails any stack segment. I think that the description in 'asdef' is out of date. I only describe the parts that I am sure about. */ struct stk_trailer { long this_address; /* Address of this block. */ long this_size; /* Size of this block (does not include this trailer). */ long unknown2; long unknown3; long link; /* Address of trailer block of previous segment. */ long unknown5; long unknown6; long unknown7; long unknown8; long unknown9; long unknown10; long unknown11; long unknown12; long unknown13; long unknown14; }; # endif /* CRAY2 */ # endif /* not CRAY_STACK */ # ifdef CRAY2 /* Determine a "stack measure" for an arbitrary ADDRESS. I doubt that "lint" will like this much. */ static long i00afunc (long *address) { struct stk_stat status; struct stk_trailer *trailer; long *block, size; long result = 0; /* We want to iterate through all of the segments. The first step is to get the stack status structure. We could do this more quickly and more directly, perhaps, by referencing the $LM00 common block, but I know that this works. */ STKSTAT (&status); /* Set up the iteration. */ trailer = (struct stk_trailer *) (status.current_address + status.current_size - 15); /* There must be at least one stack segment. Therefore it is a fatal error if "trailer" is null. */ if (trailer == 0) abort (); /* Discard segments that do not contain our argument address. */ while (trailer != 0) { block = (long *) trailer->this_address; size = trailer->this_size; if (block == 0 || size == 0) abort (); trailer = (struct stk_trailer *) trailer->link; if ((block <= address) && (address < (block + size))) break; } /* Set the result to the offset in this segment and add the sizes of all predecessor segments. */ result = address - block; if (trailer == 0) { return result; } do { if (trailer->this_size <= 0) abort (); result += trailer->this_size; trailer = (struct stk_trailer *) trailer->link; } while (trailer != 0); /* We are done. Note that if you present a bogus address (one not in any segment), you will get a different number back, formed from subtracting the address of the first block. This is probably not what you want. */ return (result); } # else /* not CRAY2 */ /* Stack address function for a CRAY-1, CRAY X-MP, or CRAY Y-MP. Determine the number of the cell within the stack, given the address of the cell. The purpose of this routine is to linearize, in some sense, stack addresses for alloca. */ static long i00afunc (long address) { long stkl = 0; long size, pseg, this_segment, stack; long result = 0; struct stack_segment_linkage *ssptr; /* Register B67 contains the address of the end of the current stack segment. If you (as a subprogram) store your registers on the stack and find that you are past the contents of B67, you have overflowed the segment. B67 also points to the stack segment linkage control area, which is what we are really interested in. */ stkl = CRAY_STACKSEG_END (); ssptr = (struct stack_segment_linkage *) stkl; /* If one subtracts 'size' from the end of the segment, one has the address of the first word of the segment. If this is not the first segment, 'pseg' will be nonzero. */ pseg = ssptr->sspseg; size = ssptr->sssize; this_segment = stkl - size; /* It is possible that calling this routine itself caused a stack overflow. Discard stack segments which do not contain the target address. */ while (!(this_segment <= address && address <= stkl)) { # ifdef DEBUG_I00AFUNC fprintf (stderr, "%011o %011o %011o\n", this_segment, address, stkl); # endif if (pseg == 0) break; stkl = stkl - pseg; ssptr = (struct stack_segment_linkage *) stkl; size = ssptr->sssize; pseg = ssptr->sspseg; this_segment = stkl - size; } result = address - this_segment; /* If you subtract pseg from the current end of the stack, you get the address of the previous stack segment's end. This seems a little convoluted to me, but I'll bet you save a cycle somewhere. */ while (pseg != 0) { # ifdef DEBUG_I00AFUNC fprintf (stderr, "%011o %011o\n", pseg, size); # endif stkl = stkl - pseg; ssptr = (struct stack_segment_linkage *) stkl; size = ssptr->sssize; pseg = ssptr->sspseg; result += size; } return (result); } # endif /* not CRAY2 */ # endif /* CRAY */ # endif /* no alloca */ #endif /* not GCC 2 */ gnuastro-0.5/bootstrapped/lib/Makefile.in0000644000175000017500000046545613217217706015514 00000000000000# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ # Copyright (C) 2002-2017 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. 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@GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = 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\ -e 's|@''REPLACE_EXPF''@|$(REPLACE_EXPF)|g' \ -e 's|@''REPLACE_EXPM1''@|$(REPLACE_EXPM1)|g' \ -e 's|@''REPLACE_EXPM1F''@|$(REPLACE_EXPM1F)|g' \ -e 's|@''REPLACE_EXP2''@|$(REPLACE_EXP2)|g' \ -e 's|@''REPLACE_EXP2L''@|$(REPLACE_EXP2L)|g' \ -e 's|@''REPLACE_FABSL''@|$(REPLACE_FABSL)|g' \ -e 's|@''REPLACE_FLOOR''@|$(REPLACE_FLOOR)|g' \ -e 's|@''REPLACE_FLOORF''@|$(REPLACE_FLOORF)|g' \ -e 's|@''REPLACE_FLOORL''@|$(REPLACE_FLOORL)|g' \ -e 's|@''REPLACE_FMA''@|$(REPLACE_FMA)|g' \ -e 's|@''REPLACE_FMAF''@|$(REPLACE_FMAF)|g' \ -e 's|@''REPLACE_FMAL''@|$(REPLACE_FMAL)|g' \ -e 's|@''REPLACE_FMOD''@|$(REPLACE_FMOD)|g' \ -e 's|@''REPLACE_FMODF''@|$(REPLACE_FMODF)|g' \ -e 's|@''REPLACE_FMODL''@|$(REPLACE_FMODL)|g' \ -e 's|@''REPLACE_FREXPF''@|$(REPLACE_FREXPF)|g' \ -e 's|@''REPLACE_FREXP''@|$(REPLACE_FREXP)|g' \ -e 's|@''REPLACE_FREXPL''@|$(REPLACE_FREXPL)|g' \ -e 's|@''REPLACE_HUGE_VAL''@|$(REPLACE_HUGE_VAL)|g' \ -e 's|@''REPLACE_HYPOT''@|$(REPLACE_HYPOT)|g' \ -e 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's|@''REPLACE_LOG2F''@|$(REPLACE_LOG2F)|g' \ -e 's|@''REPLACE_LOG2L''@|$(REPLACE_LOG2L)|g' \ -e 's|@''REPLACE_LOGB''@|$(REPLACE_LOGB)|g' \ -e 's|@''REPLACE_LOGBF''@|$(REPLACE_LOGBF)|g' \ -e 's|@''REPLACE_LOGBL''@|$(REPLACE_LOGBL)|g' \ -e 's|@''REPLACE_MODF''@|$(REPLACE_MODF)|g' \ -e 's|@''REPLACE_MODFF''@|$(REPLACE_MODFF)|g' \ -e 's|@''REPLACE_MODFL''@|$(REPLACE_MODFL)|g' \ -e 's|@''REPLACE_NAN''@|$(REPLACE_NAN)|g' \ -e 's|@''REPLACE_REMAINDER''@|$(REPLACE_REMAINDER)|g' \ -e 's|@''REPLACE_REMAINDERF''@|$(REPLACE_REMAINDERF)|g' \ -e 's|@''REPLACE_REMAINDERL''@|$(REPLACE_REMAINDERL)|g' \ -e 's|@''REPLACE_ROUND''@|$(REPLACE_ROUND)|g' \ -e 's|@''REPLACE_ROUNDF''@|$(REPLACE_ROUNDF)|g' \ -e 's|@''REPLACE_ROUNDL''@|$(REPLACE_ROUNDL)|g' \ -e 's|@''REPLACE_SIGNBIT''@|$(REPLACE_SIGNBIT)|g' \ -e 's|@''REPLACE_SIGNBIT_USING_GCC''@|$(REPLACE_SIGNBIT_USING_GCC)|g' \ -e 's|@''REPLACE_SINF''@|$(REPLACE_SINF)|g' \ -e 's|@''REPLACE_SINHF''@|$(REPLACE_SINHF)|g' \ -e 's|@''REPLACE_SQRTF''@|$(REPLACE_SQRTF)|g' \ -e 's|@''REPLACE_SQRTL''@|$(REPLACE_SQRTL)|g' \ -e 's|@''REPLACE_TANF''@|$(REPLACE_TANF)|g' \ -e 's|@''REPLACE_TANHF''@|$(REPLACE_TANHF)|g' \ -e 's|@''REPLACE_TRUNC''@|$(REPLACE_TRUNC)|g' \ -e 's|@''REPLACE_TRUNCF''@|$(REPLACE_TRUNCF)|g' \ -e 's|@''REPLACE_TRUNCL''@|$(REPLACE_TRUNCL)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works. @GL_GENERATE_STDALIGN_H_TRUE@stdalign.h: stdalign.in.h $(top_builddir)/config.status @GL_GENERATE_STDALIGN_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDALIGN_H_TRUE@ { echo '/* DO NOT EDIT! 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GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_STDBOOL_H_TRUE@ sed -e 's/@''HAVE__BOOL''@/$(HAVE__BOOL)/g' < $(srcdir)/stdbool.in.h; \ @GL_GENERATE_STDBOOL_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDBOOL_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDBOOL_H_FALSE@stdbool.h: $(top_builddir)/config.status @GL_GENERATE_STDBOOL_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. @GL_GENERATE_STDDEF_H_TRUE@stddef.h: stddef.in.h $(top_builddir)/config.status @GL_GENERATE_STDDEF_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDDEF_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ @GL_GENERATE_STDDEF_H_TRUE@ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''NEXT_STDDEF_H''@|$(NEXT_STDDEF_H)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''HAVE_MAX_ALIGN_T''@|$(HAVE_MAX_ALIGN_T)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''HAVE_WCHAR_T''@|$(HAVE_WCHAR_T)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ -e 's|@''REPLACE_NULL''@|$(REPLACE_NULL)|g' \ @GL_GENERATE_STDDEF_H_TRUE@ < $(srcdir)/stddef.in.h; \ @GL_GENERATE_STDDEF_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDDEF_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDDEF_H_FALSE@stddef.h: $(top_builddir)/config.status @GL_GENERATE_STDDEF_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. @GL_GENERATE_STDINT_H_TRUE@stdint.h: stdint.in.h $(top_builddir)/config.status @GL_GENERATE_STDINT_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_STDINT_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_STDINT_H_TRUE@ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_STDINT_H''@/$(HAVE_STDINT_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's|@''NEXT_STDINT_H''@|$(NEXT_STDINT_H)|g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_C99_STDINT_H''@/$(HAVE_C99_STDINT_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SYS_TYPES_H''@/$(HAVE_SYS_TYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_INTTYPES_H''@/$(HAVE_INTTYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SYS_INTTYPES_H''@/$(HAVE_SYS_INTTYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SYS_BITYPES_H''@/$(HAVE_SYS_BITYPES_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_WCHAR_H''@/$(HAVE_WCHAR_H)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_LONG_LONG_INT''@/$(HAVE_LONG_LONG_INT)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_UNSIGNED_LONG_LONG_INT''@/$(HAVE_UNSIGNED_LONG_LONG_INT)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''APPLE_UNIVERSAL_BUILD''@/$(APPLE_UNIVERSAL_BUILD)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_PTRDIFF_T''@/$(BITSIZEOF_PTRDIFF_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''PTRDIFF_T_SUFFIX''@/$(PTRDIFF_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_SIG_ATOMIC_T''@/$(BITSIZEOF_SIG_ATOMIC_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SIGNED_SIG_ATOMIC_T''@/$(HAVE_SIGNED_SIG_ATOMIC_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''SIG_ATOMIC_T_SUFFIX''@/$(SIG_ATOMIC_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_SIZE_T''@/$(BITSIZEOF_SIZE_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''SIZE_T_SUFFIX''@/$(SIZE_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_WCHAR_T''@/$(BITSIZEOF_WCHAR_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SIGNED_WCHAR_T''@/$(HAVE_SIGNED_WCHAR_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''WCHAR_T_SUFFIX''@/$(WCHAR_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''BITSIZEOF_WINT_T''@/$(BITSIZEOF_WINT_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''HAVE_SIGNED_WINT_T''@/$(HAVE_SIGNED_WINT_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''WINT_T_SUFFIX''@/$(WINT_T_SUFFIX)/g' \ @GL_GENERATE_STDINT_H_TRUE@ -e 's/@''GNULIB_OVERRIDES_WINT_T''@/$(GNULIB_OVERRIDES_WINT_T)/g' \ @GL_GENERATE_STDINT_H_TRUE@ < $(srcdir)/stdint.in.h; \ @GL_GENERATE_STDINT_H_TRUE@ } > $@-t && \ @GL_GENERATE_STDINT_H_TRUE@ mv $@-t $@ @GL_GENERATE_STDINT_H_FALSE@stdint.h: $(top_builddir)/config.status @GL_GENERATE_STDINT_H_FALSE@ rm -f $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdio.h: stdio.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDIO_H''@|$(NEXT_STDIO_H)|g' \ -e 's/@''GNULIB_DPRINTF''@/$(GNULIB_DPRINTF)/g' \ -e 's/@''GNULIB_FCLOSE''@/$(GNULIB_FCLOSE)/g' \ -e 's/@''GNULIB_FDOPEN''@/$(GNULIB_FDOPEN)/g' \ -e 's/@''GNULIB_FFLUSH''@/$(GNULIB_FFLUSH)/g' \ -e 's/@''GNULIB_FGETC''@/$(GNULIB_FGETC)/g' \ -e 's/@''GNULIB_FGETS''@/$(GNULIB_FGETS)/g' \ -e 's/@''GNULIB_FOPEN''@/$(GNULIB_FOPEN)/g' \ -e 's/@''GNULIB_FPRINTF''@/$(GNULIB_FPRINTF)/g' \ -e 's/@''GNULIB_FPRINTF_POSIX''@/$(GNULIB_FPRINTF_POSIX)/g' \ -e 's/@''GNULIB_FPURGE''@/$(GNULIB_FPURGE)/g' \ -e 's/@''GNULIB_FPUTC''@/$(GNULIB_FPUTC)/g' \ -e 's/@''GNULIB_FPUTS''@/$(GNULIB_FPUTS)/g' \ -e 's/@''GNULIB_FREAD''@/$(GNULIB_FREAD)/g' \ -e 's/@''GNULIB_FREOPEN''@/$(GNULIB_FREOPEN)/g' \ -e 's/@''GNULIB_FSCANF''@/$(GNULIB_FSCANF)/g' \ -e 's/@''GNULIB_FSEEK''@/$(GNULIB_FSEEK)/g' \ -e 's/@''GNULIB_FSEEKO''@/$(GNULIB_FSEEKO)/g' \ -e 's/@''GNULIB_FTELL''@/$(GNULIB_FTELL)/g' \ -e 's/@''GNULIB_FTELLO''@/$(GNULIB_FTELLO)/g' \ -e 's/@''GNULIB_FWRITE''@/$(GNULIB_FWRITE)/g' \ -e 's/@''GNULIB_GETC''@/$(GNULIB_GETC)/g' \ -e 's/@''GNULIB_GETCHAR''@/$(GNULIB_GETCHAR)/g' \ -e 's/@''GNULIB_GETDELIM''@/$(GNULIB_GETDELIM)/g' \ -e 's/@''GNULIB_GETLINE''@/$(GNULIB_GETLINE)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF''@/$(GNULIB_OBSTACK_PRINTF)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF_POSIX''@/$(GNULIB_OBSTACK_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PCLOSE''@/$(GNULIB_PCLOSE)/g' \ -e 's/@''GNULIB_PERROR''@/$(GNULIB_PERROR)/g' \ -e 's/@''GNULIB_POPEN''@/$(GNULIB_POPEN)/g' \ -e 's/@''GNULIB_PRINTF''@/$(GNULIB_PRINTF)/g' \ -e 's/@''GNULIB_PRINTF_POSIX''@/$(GNULIB_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PUTC''@/$(GNULIB_PUTC)/g' \ -e 's/@''GNULIB_PUTCHAR''@/$(GNULIB_PUTCHAR)/g' \ -e 's/@''GNULIB_PUTS''@/$(GNULIB_PUTS)/g' \ -e 's/@''GNULIB_REMOVE''@/$(GNULIB_REMOVE)/g' \ -e 's/@''GNULIB_RENAME''@/$(GNULIB_RENAME)/g' \ -e 's/@''GNULIB_RENAMEAT''@/$(GNULIB_RENAMEAT)/g' \ -e 's/@''GNULIB_SCANF''@/$(GNULIB_SCANF)/g' \ -e 's/@''GNULIB_SNPRINTF''@/$(GNULIB_SNPRINTF)/g' \ -e 's/@''GNULIB_SPRINTF_POSIX''@/$(GNULIB_SPRINTF_POSIX)/g' \ -e 's/@''GNULIB_STDIO_H_NONBLOCKING''@/$(GNULIB_STDIO_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_STDIO_H_SIGPIPE''@/$(GNULIB_STDIO_H_SIGPIPE)/g' \ -e 's/@''GNULIB_TMPFILE''@/$(GNULIB_TMPFILE)/g' \ -e 's/@''GNULIB_VASPRINTF''@/$(GNULIB_VASPRINTF)/g' \ -e 's/@''GNULIB_VDPRINTF''@/$(GNULIB_VDPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF''@/$(GNULIB_VFPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF_POSIX''@/$(GNULIB_VFPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VFSCANF''@/$(GNULIB_VFSCANF)/g' \ -e 's/@''GNULIB_VSCANF''@/$(GNULIB_VSCANF)/g' \ -e 's/@''GNULIB_VPRINTF''@/$(GNULIB_VPRINTF)/g' \ -e 's/@''GNULIB_VPRINTF_POSIX''@/$(GNULIB_VPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VSNPRINTF''@/$(GNULIB_VSNPRINTF)/g' \ -e 's/@''GNULIB_VSPRINTF_POSIX''@/$(GNULIB_VSPRINTF_POSIX)/g' \ < $(srcdir)/stdio.in.h | \ sed -e 's|@''HAVE_DECL_FPURGE''@|$(HAVE_DECL_FPURGE)|g' \ -e 's|@''HAVE_DECL_FSEEKO''@|$(HAVE_DECL_FSEEKO)|g' \ -e 's|@''HAVE_DECL_FTELLO''@|$(HAVE_DECL_FTELLO)|g' \ -e 's|@''HAVE_DECL_GETDELIM''@|$(HAVE_DECL_GETDELIM)|g' \ -e 's|@''HAVE_DECL_GETLINE''@|$(HAVE_DECL_GETLINE)|g' \ -e 's|@''HAVE_DECL_OBSTACK_PRINTF''@|$(HAVE_DECL_OBSTACK_PRINTF)|g' \ -e 's|@''HAVE_DECL_SNPRINTF''@|$(HAVE_DECL_SNPRINTF)|g' \ -e 's|@''HAVE_DECL_VSNPRINTF''@|$(HAVE_DECL_VSNPRINTF)|g' \ -e 's|@''HAVE_DPRINTF''@|$(HAVE_DPRINTF)|g' \ -e 's|@''HAVE_FSEEKO''@|$(HAVE_FSEEKO)|g' \ -e 's|@''HAVE_FTELLO''@|$(HAVE_FTELLO)|g' \ -e 's|@''HAVE_PCLOSE''@|$(HAVE_PCLOSE)|g' \ -e 's|@''HAVE_POPEN''@|$(HAVE_POPEN)|g' \ -e 's|@''HAVE_RENAMEAT''@|$(HAVE_RENAMEAT)|g' \ -e 's|@''HAVE_VASPRINTF''@|$(HAVE_VASPRINTF)|g' \ -e 's|@''HAVE_VDPRINTF''@|$(HAVE_VDPRINTF)|g' \ -e 's|@''REPLACE_DPRINTF''@|$(REPLACE_DPRINTF)|g' \ -e 's|@''REPLACE_FCLOSE''@|$(REPLACE_FCLOSE)|g' \ -e 's|@''REPLACE_FDOPEN''@|$(REPLACE_FDOPEN)|g' \ -e 's|@''REPLACE_FFLUSH''@|$(REPLACE_FFLUSH)|g' \ -e 's|@''REPLACE_FOPEN''@|$(REPLACE_FOPEN)|g' \ -e 's|@''REPLACE_FPRINTF''@|$(REPLACE_FPRINTF)|g' \ -e 's|@''REPLACE_FPURGE''@|$(REPLACE_FPURGE)|g' \ -e 's|@''REPLACE_FREOPEN''@|$(REPLACE_FREOPEN)|g' \ -e 's|@''REPLACE_FSEEK''@|$(REPLACE_FSEEK)|g' \ -e 's|@''REPLACE_FSEEKO''@|$(REPLACE_FSEEKO)|g' \ -e 's|@''REPLACE_FTELL''@|$(REPLACE_FTELL)|g' \ -e 's|@''REPLACE_FTELLO''@|$(REPLACE_FTELLO)|g' \ -e 's|@''REPLACE_GETDELIM''@|$(REPLACE_GETDELIM)|g' \ -e 's|@''REPLACE_GETLINE''@|$(REPLACE_GETLINE)|g' \ -e 's|@''REPLACE_OBSTACK_PRINTF''@|$(REPLACE_OBSTACK_PRINTF)|g' \ -e 's|@''REPLACE_PERROR''@|$(REPLACE_PERROR)|g' \ -e 's|@''REPLACE_POPEN''@|$(REPLACE_POPEN)|g' \ -e 's|@''REPLACE_PRINTF''@|$(REPLACE_PRINTF)|g' \ -e 's|@''REPLACE_REMOVE''@|$(REPLACE_REMOVE)|g' \ -e 's|@''REPLACE_RENAME''@|$(REPLACE_RENAME)|g' \ -e 's|@''REPLACE_RENAMEAT''@|$(REPLACE_RENAMEAT)|g' \ -e 's|@''REPLACE_SNPRINTF''@|$(REPLACE_SNPRINTF)|g' \ -e 's|@''REPLACE_SPRINTF''@|$(REPLACE_SPRINTF)|g' \ -e 's|@''REPLACE_STDIO_READ_FUNCS''@|$(REPLACE_STDIO_READ_FUNCS)|g' \ -e 's|@''REPLACE_STDIO_WRITE_FUNCS''@|$(REPLACE_STDIO_WRITE_FUNCS)|g' \ -e 's|@''REPLACE_TMPFILE''@|$(REPLACE_TMPFILE)|g' \ -e 's|@''REPLACE_VASPRINTF''@|$(REPLACE_VASPRINTF)|g' \ -e 's|@''REPLACE_VDPRINTF''@|$(REPLACE_VDPRINTF)|g' \ -e 's|@''REPLACE_VFPRINTF''@|$(REPLACE_VFPRINTF)|g' \ -e 's|@''REPLACE_VPRINTF''@|$(REPLACE_VPRINTF)|g' \ -e 's|@''REPLACE_VSNPRINTF''@|$(REPLACE_VSNPRINTF)|g' \ -e 's|@''REPLACE_VSPRINTF''@|$(REPLACE_VSPRINTF)|g' \ -e 's|@''ASM_SYMBOL_PREFIX''@|$(ASM_SYMBOL_PREFIX)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdlib.h: stdlib.in.h $(top_builddir)/config.status $(CXXDEFS_H) \ $(_NORETURN_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDLIB_H''@|$(NEXT_STDLIB_H)|g' \ -e 's/@''GNULIB__EXIT''@/$(GNULIB__EXIT)/g' \ -e 's/@''GNULIB_ATOLL''@/$(GNULIB_ATOLL)/g' \ -e 's/@''GNULIB_CALLOC_POSIX''@/$(GNULIB_CALLOC_POSIX)/g' \ -e 's/@''GNULIB_CANONICALIZE_FILE_NAME''@/$(GNULIB_CANONICALIZE_FILE_NAME)/g' \ -e 's/@''GNULIB_GETLOADAVG''@/$(GNULIB_GETLOADAVG)/g' \ -e 's/@''GNULIB_GETSUBOPT''@/$(GNULIB_GETSUBOPT)/g' \ -e 's/@''GNULIB_GRANTPT''@/$(GNULIB_GRANTPT)/g' \ -e 's/@''GNULIB_MALLOC_POSIX''@/$(GNULIB_MALLOC_POSIX)/g' \ -e 's/@''GNULIB_MBTOWC''@/$(GNULIB_MBTOWC)/g' \ -e 's/@''GNULIB_MKDTEMP''@/$(GNULIB_MKDTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMP''@/$(GNULIB_MKOSTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMPS''@/$(GNULIB_MKOSTEMPS)/g' \ -e 's/@''GNULIB_MKSTEMP''@/$(GNULIB_MKSTEMP)/g' \ -e 's/@''GNULIB_MKSTEMPS''@/$(GNULIB_MKSTEMPS)/g' \ -e 's/@''GNULIB_POSIX_OPENPT''@/$(GNULIB_POSIX_OPENPT)/g' \ -e 's/@''GNULIB_PTSNAME''@/$(GNULIB_PTSNAME)/g' \ -e 's/@''GNULIB_PTSNAME_R''@/$(GNULIB_PTSNAME_R)/g' \ -e 's/@''GNULIB_PUTENV''@/$(GNULIB_PUTENV)/g' \ -e 's/@''GNULIB_QSORT_R''@/$(GNULIB_QSORT_R)/g' \ -e 's/@''GNULIB_RANDOM''@/$(GNULIB_RANDOM)/g' \ -e 's/@''GNULIB_RANDOM_R''@/$(GNULIB_RANDOM_R)/g' \ -e 's/@''GNULIB_REALLOC_POSIX''@/$(GNULIB_REALLOC_POSIX)/g' \ -e 's/@''GNULIB_REALLOCARRAY''@/$(GNULIB_REALLOCARRAY)/g' \ -e 's/@''GNULIB_REALPATH''@/$(GNULIB_REALPATH)/g' \ -e 's/@''GNULIB_RPMATCH''@/$(GNULIB_RPMATCH)/g' \ -e 's/@''GNULIB_SECURE_GETENV''@/$(GNULIB_SECURE_GETENV)/g' \ -e 's/@''GNULIB_SETENV''@/$(GNULIB_SETENV)/g' \ -e 's/@''GNULIB_STRTOD''@/$(GNULIB_STRTOD)/g' \ -e 's/@''GNULIB_STRTOLL''@/$(GNULIB_STRTOLL)/g' \ -e 's/@''GNULIB_STRTOULL''@/$(GNULIB_STRTOULL)/g' \ -e 's/@''GNULIB_SYSTEM_POSIX''@/$(GNULIB_SYSTEM_POSIX)/g' \ -e 's/@''GNULIB_UNLOCKPT''@/$(GNULIB_UNLOCKPT)/g' \ -e 's/@''GNULIB_UNSETENV''@/$(GNULIB_UNSETENV)/g' \ -e 's/@''GNULIB_WCTOMB''@/$(GNULIB_WCTOMB)/g' \ < $(srcdir)/stdlib.in.h | \ sed -e 's|@''HAVE__EXIT''@|$(HAVE__EXIT)|g' \ -e 's|@''HAVE_ATOLL''@|$(HAVE_ATOLL)|g' \ -e 's|@''HAVE_CANONICALIZE_FILE_NAME''@|$(HAVE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''HAVE_DECL_GETLOADAVG''@|$(HAVE_DECL_GETLOADAVG)|g' \ -e 's|@''HAVE_GETSUBOPT''@|$(HAVE_GETSUBOPT)|g' \ -e 's|@''HAVE_GRANTPT''@|$(HAVE_GRANTPT)|g' \ -e 's|@''HAVE_DECL_INITSTATE''@|$(HAVE_DECL_INITSTATE)|g' \ -e 's|@''HAVE_MKDTEMP''@|$(HAVE_MKDTEMP)|g' \ -e 's|@''HAVE_MKOSTEMP''@|$(HAVE_MKOSTEMP)|g' \ -e 's|@''HAVE_MKOSTEMPS''@|$(HAVE_MKOSTEMPS)|g' \ -e 's|@''HAVE_MKSTEMP''@|$(HAVE_MKSTEMP)|g' \ -e 's|@''HAVE_MKSTEMPS''@|$(HAVE_MKSTEMPS)|g' \ -e 's|@''HAVE_POSIX_OPENPT''@|$(HAVE_POSIX_OPENPT)|g' \ -e 's|@''HAVE_PTSNAME''@|$(HAVE_PTSNAME)|g' \ -e 's|@''HAVE_PTSNAME_R''@|$(HAVE_PTSNAME_R)|g' \ -e 's|@''HAVE_QSORT_R''@|$(HAVE_QSORT_R)|g' \ -e 's|@''HAVE_RANDOM''@|$(HAVE_RANDOM)|g' \ -e 's|@''HAVE_RANDOM_H''@|$(HAVE_RANDOM_H)|g' \ -e 's|@''HAVE_RANDOM_R''@|$(HAVE_RANDOM_R)|g' \ -e 's|@''HAVE_REALLOCARRAY''@|$(HAVE_REALLOCARRAY)|g' \ -e 's|@''HAVE_REALPATH''@|$(HAVE_REALPATH)|g' \ -e 's|@''HAVE_RPMATCH''@|$(HAVE_RPMATCH)|g' \ -e 's|@''HAVE_SECURE_GETENV''@|$(HAVE_SECURE_GETENV)|g' \ -e 's|@''HAVE_DECL_SETENV''@|$(HAVE_DECL_SETENV)|g' \ -e 's|@''HAVE_DECL_SETSTATE''@|$(HAVE_DECL_SETSTATE)|g' \ -e 's|@''HAVE_STRTOD''@|$(HAVE_STRTOD)|g' \ -e 's|@''HAVE_STRTOLL''@|$(HAVE_STRTOLL)|g' \ -e 's|@''HAVE_STRTOULL''@|$(HAVE_STRTOULL)|g' \ -e 's|@''HAVE_STRUCT_RANDOM_DATA''@|$(HAVE_STRUCT_RANDOM_DATA)|g' \ -e 's|@''HAVE_SYS_LOADAVG_H''@|$(HAVE_SYS_LOADAVG_H)|g' \ -e 's|@''HAVE_UNLOCKPT''@|$(HAVE_UNLOCKPT)|g' \ -e 's|@''HAVE_DECL_UNSETENV''@|$(HAVE_DECL_UNSETENV)|g' \ -e 's|@''REPLACE_CALLOC''@|$(REPLACE_CALLOC)|g' \ -e 's|@''REPLACE_CANONICALIZE_FILE_NAME''@|$(REPLACE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''REPLACE_MALLOC''@|$(REPLACE_MALLOC)|g' \ -e 's|@''REPLACE_MBTOWC''@|$(REPLACE_MBTOWC)|g' \ -e 's|@''REPLACE_MKSTEMP''@|$(REPLACE_MKSTEMP)|g' \ -e 's|@''REPLACE_PTSNAME''@|$(REPLACE_PTSNAME)|g' \ -e 's|@''REPLACE_PTSNAME_R''@|$(REPLACE_PTSNAME_R)|g' \ -e 's|@''REPLACE_PUTENV''@|$(REPLACE_PUTENV)|g' \ -e 's|@''REPLACE_QSORT_R''@|$(REPLACE_QSORT_R)|g' \ -e 's|@''REPLACE_RANDOM_R''@|$(REPLACE_RANDOM_R)|g' \ -e 's|@''REPLACE_REALLOC''@|$(REPLACE_REALLOC)|g' \ -e 's|@''REPLACE_REALPATH''@|$(REPLACE_REALPATH)|g' \ -e 's|@''REPLACE_SETENV''@|$(REPLACE_SETENV)|g' \ -e 's|@''REPLACE_STRTOD''@|$(REPLACE_STRTOD)|g' \ -e 's|@''REPLACE_UNSETENV''@|$(REPLACE_UNSETENV)|g' \ -e 's|@''REPLACE_WCTOMB''@|$(REPLACE_WCTOMB)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _Noreturn/r $(_NORETURN_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. string.h: string.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRING_H''@|$(NEXT_STRING_H)|g' \ -e 's/@''GNULIB_EXPLICIT_BZERO''@/$(GNULIB_EXPLICIT_BZERO)/g' \ -e 's/@''GNULIB_FFSL''@/$(GNULIB_FFSL)/g' \ -e 's/@''GNULIB_FFSLL''@/$(GNULIB_FFSLL)/g' \ -e 's/@''GNULIB_MBSLEN''@/$(GNULIB_MBSLEN)/g' \ -e 's/@''GNULIB_MBSNLEN''@/$(GNULIB_MBSNLEN)/g' \ -e 's/@''GNULIB_MBSCHR''@/$(GNULIB_MBSCHR)/g' \ -e 's/@''GNULIB_MBSRCHR''@/$(GNULIB_MBSRCHR)/g' \ -e 's/@''GNULIB_MBSSTR''@/$(GNULIB_MBSSTR)/g' \ -e 's/@''GNULIB_MBSCASECMP''@/$(GNULIB_MBSCASECMP)/g' \ -e 's/@''GNULIB_MBSNCASECMP''@/$(GNULIB_MBSNCASECMP)/g' \ -e 's/@''GNULIB_MBSPCASECMP''@/$(GNULIB_MBSPCASECMP)/g' \ -e 's/@''GNULIB_MBSCASESTR''@/$(GNULIB_MBSCASESTR)/g' \ -e 's/@''GNULIB_MBSCSPN''@/$(GNULIB_MBSCSPN)/g' \ -e 's/@''GNULIB_MBSPBRK''@/$(GNULIB_MBSPBRK)/g' \ -e 's/@''GNULIB_MBSSPN''@/$(GNULIB_MBSSPN)/g' \ -e 's/@''GNULIB_MBSSEP''@/$(GNULIB_MBSSEP)/g' \ -e 's/@''GNULIB_MBSTOK_R''@/$(GNULIB_MBSTOK_R)/g' \ -e 's/@''GNULIB_MEMCHR''@/$(GNULIB_MEMCHR)/g' \ -e 's/@''GNULIB_MEMMEM''@/$(GNULIB_MEMMEM)/g' \ -e 's/@''GNULIB_MEMPCPY''@/$(GNULIB_MEMPCPY)/g' \ -e 's/@''GNULIB_MEMRCHR''@/$(GNULIB_MEMRCHR)/g' \ -e 's/@''GNULIB_RAWMEMCHR''@/$(GNULIB_RAWMEMCHR)/g' \ -e 's/@''GNULIB_STPCPY''@/$(GNULIB_STPCPY)/g' \ -e 's/@''GNULIB_STPNCPY''@/$(GNULIB_STPNCPY)/g' \ -e 's/@''GNULIB_STRCHRNUL''@/$(GNULIB_STRCHRNUL)/g' \ -e 's/@''GNULIB_STRDUP''@/$(GNULIB_STRDUP)/g' \ -e 's/@''GNULIB_STRNCAT''@/$(GNULIB_STRNCAT)/g' \ -e 's/@''GNULIB_STRNDUP''@/$(GNULIB_STRNDUP)/g' \ -e 's/@''GNULIB_STRNLEN''@/$(GNULIB_STRNLEN)/g' \ -e 's/@''GNULIB_STRPBRK''@/$(GNULIB_STRPBRK)/g' \ -e 's/@''GNULIB_STRSEP''@/$(GNULIB_STRSEP)/g' \ -e 's/@''GNULIB_STRSTR''@/$(GNULIB_STRSTR)/g' \ -e 's/@''GNULIB_STRCASESTR''@/$(GNULIB_STRCASESTR)/g' \ -e 's/@''GNULIB_STRTOK_R''@/$(GNULIB_STRTOK_R)/g' \ -e 's/@''GNULIB_STRERROR''@/$(GNULIB_STRERROR)/g' \ -e 's/@''GNULIB_STRERROR_R''@/$(GNULIB_STRERROR_R)/g' \ -e 's/@''GNULIB_STRSIGNAL''@/$(GNULIB_STRSIGNAL)/g' \ -e 's/@''GNULIB_STRVERSCMP''@/$(GNULIB_STRVERSCMP)/g' \ < $(srcdir)/string.in.h | \ sed -e 's|@''HAVE_EXPLICIT_BZERO''@|$(HAVE_EXPLICIT_BZERO)|g' \ -e 's|@''HAVE_FFSL''@|$(HAVE_FFSL)|g' \ -e 's|@''HAVE_FFSLL''@|$(HAVE_FFSLL)|g' \ -e 's|@''HAVE_MBSLEN''@|$(HAVE_MBSLEN)|g' \ -e 's|@''HAVE_MEMCHR''@|$(HAVE_MEMCHR)|g' \ -e 's|@''HAVE_DECL_MEMMEM''@|$(HAVE_DECL_MEMMEM)|g' \ -e 's|@''HAVE_MEMPCPY''@|$(HAVE_MEMPCPY)|g' \ -e 's|@''HAVE_DECL_MEMRCHR''@|$(HAVE_DECL_MEMRCHR)|g' \ -e 's|@''HAVE_RAWMEMCHR''@|$(HAVE_RAWMEMCHR)|g' \ -e 's|@''HAVE_STPCPY''@|$(HAVE_STPCPY)|g' \ -e 's|@''HAVE_STPNCPY''@|$(HAVE_STPNCPY)|g' \ -e 's|@''HAVE_STRCHRNUL''@|$(HAVE_STRCHRNUL)|g' \ -e 's|@''HAVE_DECL_STRDUP''@|$(HAVE_DECL_STRDUP)|g' \ -e 's|@''HAVE_DECL_STRNDUP''@|$(HAVE_DECL_STRNDUP)|g' \ -e 's|@''HAVE_DECL_STRNLEN''@|$(HAVE_DECL_STRNLEN)|g' \ -e 's|@''HAVE_STRPBRK''@|$(HAVE_STRPBRK)|g' \ -e 's|@''HAVE_STRSEP''@|$(HAVE_STRSEP)|g' \ -e 's|@''HAVE_STRCASESTR''@|$(HAVE_STRCASESTR)|g' \ -e 's|@''HAVE_DECL_STRTOK_R''@|$(HAVE_DECL_STRTOK_R)|g' \ -e 's|@''HAVE_DECL_STRERROR_R''@|$(HAVE_DECL_STRERROR_R)|g' \ -e 's|@''HAVE_DECL_STRSIGNAL''@|$(HAVE_DECL_STRSIGNAL)|g' \ -e 's|@''HAVE_STRVERSCMP''@|$(HAVE_STRVERSCMP)|g' \ -e 's|@''REPLACE_MEMCHR''@|$(REPLACE_MEMCHR)|g' \ -e 's|@''REPLACE_MEMMEM''@|$(REPLACE_MEMMEM)|g' \ -e 's|@''REPLACE_STPNCPY''@|$(REPLACE_STPNCPY)|g' \ -e 's|@''REPLACE_STRCHRNUL''@|$(REPLACE_STRCHRNUL)|g' \ -e 's|@''REPLACE_STRDUP''@|$(REPLACE_STRDUP)|g' \ -e 's|@''REPLACE_STRNCAT''@|$(REPLACE_STRNCAT)|g' \ -e 's|@''REPLACE_STRNDUP''@|$(REPLACE_STRNDUP)|g' \ -e 's|@''REPLACE_STRNLEN''@|$(REPLACE_STRNLEN)|g' \ -e 's|@''REPLACE_STRSTR''@|$(REPLACE_STRSTR)|g' \ -e 's|@''REPLACE_STRCASESTR''@|$(REPLACE_STRCASESTR)|g' \ -e 's|@''REPLACE_STRTOK_R''@|$(REPLACE_STRTOK_R)|g' \ -e 's|@''REPLACE_STRERROR''@|$(REPLACE_STRERROR)|g' \ -e 's|@''REPLACE_STRERROR_R''@|$(REPLACE_STRERROR_R)|g' \ -e 's|@''REPLACE_STRSIGNAL''@|$(REPLACE_STRSIGNAL)|g' \ -e 's|@''UNDEFINE_STRTOK_R''@|$(UNDEFINE_STRTOK_R)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ < $(srcdir)/string.in.h; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. strings.h: strings.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_STRINGS_H''@|$(HAVE_STRINGS_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRINGS_H''@|$(NEXT_STRINGS_H)|g' \ -e 's|@''GNULIB_FFS''@|$(GNULIB_FFS)|g' \ -e 's|@''HAVE_FFS''@|$(HAVE_FFS)|g' \ -e 's|@''HAVE_STRCASECMP''@|$(HAVE_STRCASECMP)|g' \ -e 's|@''HAVE_DECL_STRNCASECMP''@|$(HAVE_DECL_STRNCASECMP)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/strings.in.h; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/types.h: sys_types.in.h $(top_builddir)/config.status $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_TYPES_H''@|$(NEXT_SYS_TYPES_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ -e 's|@''WINDOWS_STAT_INODES''@|$(WINDOWS_STAT_INODES)|g' \ < $(srcdir)/sys_types.in.h; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. @GL_GENERATE_SYSEXITS_H_TRUE@sysexits.h: sysexits.in.h $(top_builddir)/config.status @GL_GENERATE_SYSEXITS_H_TRUE@ $(AM_V_GEN)rm -f $@-t $@ && \ @GL_GENERATE_SYSEXITS_H_TRUE@ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ @GL_GENERATE_SYSEXITS_H_TRUE@ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''HAVE_SYSEXITS_H''@|$(HAVE_SYSEXITS_H)|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ -e 's|@''NEXT_SYSEXITS_H''@|$(NEXT_SYSEXITS_H)|g' \ @GL_GENERATE_SYSEXITS_H_TRUE@ < $(srcdir)/sysexits.in.h; \ @GL_GENERATE_SYSEXITS_H_TRUE@ } > $@-t && \ @GL_GENERATE_SYSEXITS_H_TRUE@ mv -f $@-t $@ @GL_GENERATE_SYSEXITS_H_FALSE@sysexits.h: $(top_builddir)/config.status @GL_GENERATE_SYSEXITS_H_FALSE@ rm -f $@ # We need the following in order to create an empty placeholder for # when the system doesn't have one. unistd.h: unistd.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_UNISTD_H''@|$(HAVE_UNISTD_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_UNISTD_H''@|$(NEXT_UNISTD_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ -e 's/@''GNULIB_CHDIR''@/$(GNULIB_CHDIR)/g' \ -e 's/@''GNULIB_CHOWN''@/$(GNULIB_CHOWN)/g' \ -e 's/@''GNULIB_CLOSE''@/$(GNULIB_CLOSE)/g' \ -e 's/@''GNULIB_DUP''@/$(GNULIB_DUP)/g' \ -e 's/@''GNULIB_DUP2''@/$(GNULIB_DUP2)/g' \ -e 's/@''GNULIB_DUP3''@/$(GNULIB_DUP3)/g' \ -e 's/@''GNULIB_ENVIRON''@/$(GNULIB_ENVIRON)/g' \ -e 's/@''GNULIB_EUIDACCESS''@/$(GNULIB_EUIDACCESS)/g' \ -e 's/@''GNULIB_FACCESSAT''@/$(GNULIB_FACCESSAT)/g' \ -e 's/@''GNULIB_FCHDIR''@/$(GNULIB_FCHDIR)/g' \ -e 's/@''GNULIB_FCHOWNAT''@/$(GNULIB_FCHOWNAT)/g' \ -e 's/@''GNULIB_FDATASYNC''@/$(GNULIB_FDATASYNC)/g' \ -e 's/@''GNULIB_FSYNC''@/$(GNULIB_FSYNC)/g' \ -e 's/@''GNULIB_FTRUNCATE''@/$(GNULIB_FTRUNCATE)/g' \ -e 's/@''GNULIB_GETCWD''@/$(GNULIB_GETCWD)/g' \ -e 's/@''GNULIB_GETDOMAINNAME''@/$(GNULIB_GETDOMAINNAME)/g' \ -e 's/@''GNULIB_GETDTABLESIZE''@/$(GNULIB_GETDTABLESIZE)/g' \ -e 's/@''GNULIB_GETGROUPS''@/$(GNULIB_GETGROUPS)/g' \ -e 's/@''GNULIB_GETHOSTNAME''@/$(GNULIB_GETHOSTNAME)/g' \ -e 's/@''GNULIB_GETLOGIN''@/$(GNULIB_GETLOGIN)/g' \ -e 's/@''GNULIB_GETLOGIN_R''@/$(GNULIB_GETLOGIN_R)/g' \ -e 's/@''GNULIB_GETPAGESIZE''@/$(GNULIB_GETPAGESIZE)/g' \ -e 's/@''GNULIB_GETUSERSHELL''@/$(GNULIB_GETUSERSHELL)/g' \ -e 's/@''GNULIB_GROUP_MEMBER''@/$(GNULIB_GROUP_MEMBER)/g' \ -e 's/@''GNULIB_ISATTY''@/$(GNULIB_ISATTY)/g' \ -e 's/@''GNULIB_LCHOWN''@/$(GNULIB_LCHOWN)/g' \ -e 's/@''GNULIB_LINK''@/$(GNULIB_LINK)/g' \ -e 's/@''GNULIB_LINKAT''@/$(GNULIB_LINKAT)/g' \ -e 's/@''GNULIB_LSEEK''@/$(GNULIB_LSEEK)/g' \ -e 's/@''GNULIB_PIPE''@/$(GNULIB_PIPE)/g' \ -e 's/@''GNULIB_PIPE2''@/$(GNULIB_PIPE2)/g' \ -e 's/@''GNULIB_PREAD''@/$(GNULIB_PREAD)/g' \ -e 's/@''GNULIB_PWRITE''@/$(GNULIB_PWRITE)/g' \ -e 's/@''GNULIB_READ''@/$(GNULIB_READ)/g' \ -e 's/@''GNULIB_READLINK''@/$(GNULIB_READLINK)/g' \ -e 's/@''GNULIB_READLINKAT''@/$(GNULIB_READLINKAT)/g' \ -e 's/@''GNULIB_RMDIR''@/$(GNULIB_RMDIR)/g' \ -e 's/@''GNULIB_SETHOSTNAME''@/$(GNULIB_SETHOSTNAME)/g' \ -e 's/@''GNULIB_SLEEP''@/$(GNULIB_SLEEP)/g' \ -e 's/@''GNULIB_SYMLINK''@/$(GNULIB_SYMLINK)/g' \ -e 's/@''GNULIB_SYMLINKAT''@/$(GNULIB_SYMLINKAT)/g' \ -e 's/@''GNULIB_TRUNCATE''@/$(GNULIB_TRUNCATE)/g' \ -e 's/@''GNULIB_TTYNAME_R''@/$(GNULIB_TTYNAME_R)/g' \ -e 's/@''GNULIB_UNISTD_H_GETOPT''@/0$(GNULIB_GL_UNISTD_H_GETOPT)/g' \ -e 's/@''GNULIB_UNISTD_H_NONBLOCKING''@/$(GNULIB_UNISTD_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_UNISTD_H_SIGPIPE''@/$(GNULIB_UNISTD_H_SIGPIPE)/g' \ -e 's/@''GNULIB_UNLINK''@/$(GNULIB_UNLINK)/g' \ -e 's/@''GNULIB_UNLINKAT''@/$(GNULIB_UNLINKAT)/g' \ -e 's/@''GNULIB_USLEEP''@/$(GNULIB_USLEEP)/g' \ -e 's/@''GNULIB_WRITE''@/$(GNULIB_WRITE)/g' \ < $(srcdir)/unistd.in.h | \ sed -e 's|@''HAVE_CHOWN''@|$(HAVE_CHOWN)|g' \ -e 's|@''HAVE_DUP2''@|$(HAVE_DUP2)|g' \ -e 's|@''HAVE_DUP3''@|$(HAVE_DUP3)|g' \ -e 's|@''HAVE_EUIDACCESS''@|$(HAVE_EUIDACCESS)|g' \ -e 's|@''HAVE_FACCESSAT''@|$(HAVE_FACCESSAT)|g' \ -e 's|@''HAVE_FCHDIR''@|$(HAVE_FCHDIR)|g' \ -e 's|@''HAVE_FCHOWNAT''@|$(HAVE_FCHOWNAT)|g' \ -e 's|@''HAVE_FDATASYNC''@|$(HAVE_FDATASYNC)|g' \ -e 's|@''HAVE_FSYNC''@|$(HAVE_FSYNC)|g' \ -e 's|@''HAVE_FTRUNCATE''@|$(HAVE_FTRUNCATE)|g' \ -e 's|@''HAVE_GETDTABLESIZE''@|$(HAVE_GETDTABLESIZE)|g' \ -e 's|@''HAVE_GETGROUPS''@|$(HAVE_GETGROUPS)|g' \ -e 's|@''HAVE_GETHOSTNAME''@|$(HAVE_GETHOSTNAME)|g' \ -e 's|@''HAVE_GETPAGESIZE''@|$(HAVE_GETPAGESIZE)|g' \ -e 's|@''HAVE_GROUP_MEMBER''@|$(HAVE_GROUP_MEMBER)|g' \ -e 's|@''HAVE_LCHOWN''@|$(HAVE_LCHOWN)|g' \ -e 's|@''HAVE_LINK''@|$(HAVE_LINK)|g' \ -e 's|@''HAVE_LINKAT''@|$(HAVE_LINKAT)|g' \ -e 's|@''HAVE_PIPE''@|$(HAVE_PIPE)|g' \ -e 's|@''HAVE_PIPE2''@|$(HAVE_PIPE2)|g' \ -e 's|@''HAVE_PREAD''@|$(HAVE_PREAD)|g' \ -e 's|@''HAVE_PWRITE''@|$(HAVE_PWRITE)|g' \ -e 's|@''HAVE_READLINK''@|$(HAVE_READLINK)|g' \ -e 's|@''HAVE_READLINKAT''@|$(HAVE_READLINKAT)|g' \ -e 's|@''HAVE_SETHOSTNAME''@|$(HAVE_SETHOSTNAME)|g' \ -e 's|@''HAVE_SLEEP''@|$(HAVE_SLEEP)|g' \ -e 's|@''HAVE_SYMLINK''@|$(HAVE_SYMLINK)|g' \ -e 's|@''HAVE_SYMLINKAT''@|$(HAVE_SYMLINKAT)|g' \ -e 's|@''HAVE_TRUNCATE''@|$(HAVE_TRUNCATE)|g' \ -e 's|@''HAVE_UNLINKAT''@|$(HAVE_UNLINKAT)|g' \ -e 's|@''HAVE_USLEEP''@|$(HAVE_USLEEP)|g' \ -e 's|@''HAVE_DECL_ENVIRON''@|$(HAVE_DECL_ENVIRON)|g' \ -e 's|@''HAVE_DECL_FCHDIR''@|$(HAVE_DECL_FCHDIR)|g' \ -e 's|@''HAVE_DECL_FDATASYNC''@|$(HAVE_DECL_FDATASYNC)|g' \ -e 's|@''HAVE_DECL_GETDOMAINNAME''@|$(HAVE_DECL_GETDOMAINNAME)|g' \ -e 's|@''HAVE_DECL_GETLOGIN''@|$(HAVE_DECL_GETLOGIN)|g' \ -e 's|@''HAVE_DECL_GETLOGIN_R''@|$(HAVE_DECL_GETLOGIN_R)|g' \ -e 's|@''HAVE_DECL_GETPAGESIZE''@|$(HAVE_DECL_GETPAGESIZE)|g' \ -e 's|@''HAVE_DECL_GETUSERSHELL''@|$(HAVE_DECL_GETUSERSHELL)|g' \ -e 's|@''HAVE_DECL_SETHOSTNAME''@|$(HAVE_DECL_SETHOSTNAME)|g' \ -e 's|@''HAVE_DECL_TTYNAME_R''@|$(HAVE_DECL_TTYNAME_R)|g' \ -e 's|@''HAVE_OS_H''@|$(HAVE_OS_H)|g' \ -e 's|@''HAVE_SYS_PARAM_H''@|$(HAVE_SYS_PARAM_H)|g' \ | \ sed -e 's|@''REPLACE_CHOWN''@|$(REPLACE_CHOWN)|g' \ -e 's|@''REPLACE_CLOSE''@|$(REPLACE_CLOSE)|g' \ -e 's|@''REPLACE_DUP''@|$(REPLACE_DUP)|g' \ -e 's|@''REPLACE_DUP2''@|$(REPLACE_DUP2)|g' \ -e 's|@''REPLACE_FACCESSAT''@|$(REPLACE_FACCESSAT)|g' \ -e 's|@''REPLACE_FCHOWNAT''@|$(REPLACE_FCHOWNAT)|g' \ -e 's|@''REPLACE_FTRUNCATE''@|$(REPLACE_FTRUNCATE)|g' \ -e 's|@''REPLACE_GETCWD''@|$(REPLACE_GETCWD)|g' \ -e 's|@''REPLACE_GETDOMAINNAME''@|$(REPLACE_GETDOMAINNAME)|g' \ -e 's|@''REPLACE_GETDTABLESIZE''@|$(REPLACE_GETDTABLESIZE)|g' \ -e 's|@''REPLACE_GETLOGIN_R''@|$(REPLACE_GETLOGIN_R)|g' \ -e 's|@''REPLACE_GETGROUPS''@|$(REPLACE_GETGROUPS)|g' \ -e 's|@''REPLACE_GETPAGESIZE''@|$(REPLACE_GETPAGESIZE)|g' \ -e 's|@''REPLACE_ISATTY''@|$(REPLACE_ISATTY)|g' \ -e 's|@''REPLACE_LCHOWN''@|$(REPLACE_LCHOWN)|g' \ -e 's|@''REPLACE_LINK''@|$(REPLACE_LINK)|g' \ -e 's|@''REPLACE_LINKAT''@|$(REPLACE_LINKAT)|g' \ -e 's|@''REPLACE_LSEEK''@|$(REPLACE_LSEEK)|g' \ -e 's|@''REPLACE_PREAD''@|$(REPLACE_PREAD)|g' \ -e 's|@''REPLACE_PWRITE''@|$(REPLACE_PWRITE)|g' \ -e 's|@''REPLACE_READ''@|$(REPLACE_READ)|g' \ -e 's|@''REPLACE_READLINK''@|$(REPLACE_READLINK)|g' \ -e 's|@''REPLACE_READLINKAT''@|$(REPLACE_READLINKAT)|g' \ -e 's|@''REPLACE_RMDIR''@|$(REPLACE_RMDIR)|g' \ -e 's|@''REPLACE_SLEEP''@|$(REPLACE_SLEEP)|g' \ -e 's|@''REPLACE_SYMLINK''@|$(REPLACE_SYMLINK)|g' \ -e 's|@''REPLACE_SYMLINKAT''@|$(REPLACE_SYMLINKAT)|g' \ -e 's|@''REPLACE_TRUNCATE''@|$(REPLACE_TRUNCATE)|g' \ -e 's|@''REPLACE_TTYNAME_R''@|$(REPLACE_TTYNAME_R)|g' \ -e 's|@''REPLACE_UNLINK''@|$(REPLACE_UNLINK)|g' \ -e 's|@''REPLACE_UNLINKAT''@|$(REPLACE_UNLINKAT)|g' \ -e 's|@''REPLACE_USLEEP''@|$(REPLACE_USLEEP)|g' \ -e 's|@''REPLACE_WRITE''@|$(REPLACE_WRITE)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H''@|$(UNISTD_H_HAVE_WINSOCK2_H)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS''@|$(UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ unitypes.h: unitypes.in.h $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/unitypes.in.h; \ } > $@-t && \ mv -f $@-t $@ uniwidth.h: uniwidth.in.h $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/uniwidth.in.h; \ } > $@-t && \ mv -f $@-t $@ # We need the following in order to create when the system # version does not work standalone. wchar.h: wchar.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''HAVE_FEATURES_H''@|$(HAVE_FEATURES_H)|g' \ -e 's|@''NEXT_WCHAR_H''@|$(NEXT_WCHAR_H)|g' \ -e 's|@''HAVE_WCHAR_H''@|$(HAVE_WCHAR_H)|g' \ -e 's/@''HAVE_CRTDEFS_H''@/$(HAVE_CRTDEFS_H)/g' \ -e 's/@''GNULIB_OVERRIDES_WINT_T''@/$(GNULIB_OVERRIDES_WINT_T)/g' \ -e 's/@''GNULIB_BTOWC''@/$(GNULIB_BTOWC)/g' \ -e 's/@''GNULIB_WCTOB''@/$(GNULIB_WCTOB)/g' \ -e 's/@''GNULIB_MBSINIT''@/$(GNULIB_MBSINIT)/g' \ -e 's/@''GNULIB_MBRTOWC''@/$(GNULIB_MBRTOWC)/g' \ -e 's/@''GNULIB_MBRLEN''@/$(GNULIB_MBRLEN)/g' \ -e 's/@''GNULIB_MBSRTOWCS''@/$(GNULIB_MBSRTOWCS)/g' \ -e 's/@''GNULIB_MBSNRTOWCS''@/$(GNULIB_MBSNRTOWCS)/g' \ -e 's/@''GNULIB_WCRTOMB''@/$(GNULIB_WCRTOMB)/g' \ -e 's/@''GNULIB_WCSRTOMBS''@/$(GNULIB_WCSRTOMBS)/g' \ -e 's/@''GNULIB_WCSNRTOMBS''@/$(GNULIB_WCSNRTOMBS)/g' \ -e 's/@''GNULIB_WCWIDTH''@/$(GNULIB_WCWIDTH)/g' \ -e 's/@''GNULIB_WMEMCHR''@/$(GNULIB_WMEMCHR)/g' \ -e 's/@''GNULIB_WMEMCMP''@/$(GNULIB_WMEMCMP)/g' \ -e 's/@''GNULIB_WMEMCPY''@/$(GNULIB_WMEMCPY)/g' \ -e 's/@''GNULIB_WMEMMOVE''@/$(GNULIB_WMEMMOVE)/g' \ -e 's/@''GNULIB_WMEMSET''@/$(GNULIB_WMEMSET)/g' \ -e 's/@''GNULIB_WCSLEN''@/$(GNULIB_WCSLEN)/g' \ -e 's/@''GNULIB_WCSNLEN''@/$(GNULIB_WCSNLEN)/g' \ -e 's/@''GNULIB_WCSCPY''@/$(GNULIB_WCSCPY)/g' \ -e 's/@''GNULIB_WCPCPY''@/$(GNULIB_WCPCPY)/g' \ -e 's/@''GNULIB_WCSNCPY''@/$(GNULIB_WCSNCPY)/g' \ -e 's/@''GNULIB_WCPNCPY''@/$(GNULIB_WCPNCPY)/g' \ -e 's/@''GNULIB_WCSCAT''@/$(GNULIB_WCSCAT)/g' \ -e 's/@''GNULIB_WCSNCAT''@/$(GNULIB_WCSNCAT)/g' \ -e 's/@''GNULIB_WCSCMP''@/$(GNULIB_WCSCMP)/g' \ -e 's/@''GNULIB_WCSNCMP''@/$(GNULIB_WCSNCMP)/g' \ -e 's/@''GNULIB_WCSCASECMP''@/$(GNULIB_WCSCASECMP)/g' \ -e 's/@''GNULIB_WCSNCASECMP''@/$(GNULIB_WCSNCASECMP)/g' \ -e 's/@''GNULIB_WCSCOLL''@/$(GNULIB_WCSCOLL)/g' \ -e 's/@''GNULIB_WCSXFRM''@/$(GNULIB_WCSXFRM)/g' \ -e 's/@''GNULIB_WCSDUP''@/$(GNULIB_WCSDUP)/g' \ -e 's/@''GNULIB_WCSCHR''@/$(GNULIB_WCSCHR)/g' \ -e 's/@''GNULIB_WCSRCHR''@/$(GNULIB_WCSRCHR)/g' \ -e 's/@''GNULIB_WCSCSPN''@/$(GNULIB_WCSCSPN)/g' \ -e 's/@''GNULIB_WCSSPN''@/$(GNULIB_WCSSPN)/g' \ -e 's/@''GNULIB_WCSPBRK''@/$(GNULIB_WCSPBRK)/g' \ -e 's/@''GNULIB_WCSSTR''@/$(GNULIB_WCSSTR)/g' \ -e 's/@''GNULIB_WCSTOK''@/$(GNULIB_WCSTOK)/g' \ -e 's/@''GNULIB_WCSWIDTH''@/$(GNULIB_WCSWIDTH)/g' \ -e 's/@''GNULIB_WCSFTIME''@/$(GNULIB_WCSFTIME)/g' \ < $(srcdir)/wchar.in.h | \ sed -e 's|@''HAVE_WINT_T''@|$(HAVE_WINT_T)|g' \ -e 's|@''HAVE_BTOWC''@|$(HAVE_BTOWC)|g' \ -e 's|@''HAVE_MBSINIT''@|$(HAVE_MBSINIT)|g' \ -e 's|@''HAVE_MBRTOWC''@|$(HAVE_MBRTOWC)|g' \ -e 's|@''HAVE_MBRLEN''@|$(HAVE_MBRLEN)|g' \ -e 's|@''HAVE_MBSRTOWCS''@|$(HAVE_MBSRTOWCS)|g' \ -e 's|@''HAVE_MBSNRTOWCS''@|$(HAVE_MBSNRTOWCS)|g' \ -e 's|@''HAVE_WCRTOMB''@|$(HAVE_WCRTOMB)|g' \ -e 's|@''HAVE_WCSRTOMBS''@|$(HAVE_WCSRTOMBS)|g' \ -e 's|@''HAVE_WCSNRTOMBS''@|$(HAVE_WCSNRTOMBS)|g' \ -e 's|@''HAVE_WMEMCHR''@|$(HAVE_WMEMCHR)|g' \ -e 's|@''HAVE_WMEMCMP''@|$(HAVE_WMEMCMP)|g' \ -e 's|@''HAVE_WMEMCPY''@|$(HAVE_WMEMCPY)|g' \ -e 's|@''HAVE_WMEMMOVE''@|$(HAVE_WMEMMOVE)|g' \ -e 's|@''HAVE_WMEMSET''@|$(HAVE_WMEMSET)|g' \ -e 's|@''HAVE_WCSLEN''@|$(HAVE_WCSLEN)|g' \ -e 's|@''HAVE_WCSNLEN''@|$(HAVE_WCSNLEN)|g' \ -e 's|@''HAVE_WCSCPY''@|$(HAVE_WCSCPY)|g' \ -e 's|@''HAVE_WCPCPY''@|$(HAVE_WCPCPY)|g' \ -e 's|@''HAVE_WCSNCPY''@|$(HAVE_WCSNCPY)|g' \ -e 's|@''HAVE_WCPNCPY''@|$(HAVE_WCPNCPY)|g' \ -e 's|@''HAVE_WCSCAT''@|$(HAVE_WCSCAT)|g' \ -e 's|@''HAVE_WCSNCAT''@|$(HAVE_WCSNCAT)|g' \ -e 's|@''HAVE_WCSCMP''@|$(HAVE_WCSCMP)|g' \ -e 's|@''HAVE_WCSNCMP''@|$(HAVE_WCSNCMP)|g' \ -e 's|@''HAVE_WCSCASECMP''@|$(HAVE_WCSCASECMP)|g' \ -e 's|@''HAVE_WCSNCASECMP''@|$(HAVE_WCSNCASECMP)|g' \ -e 's|@''HAVE_WCSCOLL''@|$(HAVE_WCSCOLL)|g' \ -e 's|@''HAVE_WCSXFRM''@|$(HAVE_WCSXFRM)|g' \ -e 's|@''HAVE_WCSDUP''@|$(HAVE_WCSDUP)|g' \ -e 's|@''HAVE_WCSCHR''@|$(HAVE_WCSCHR)|g' \ -e 's|@''HAVE_WCSRCHR''@|$(HAVE_WCSRCHR)|g' \ -e 's|@''HAVE_WCSCSPN''@|$(HAVE_WCSCSPN)|g' \ -e 's|@''HAVE_WCSSPN''@|$(HAVE_WCSSPN)|g' \ -e 's|@''HAVE_WCSPBRK''@|$(HAVE_WCSPBRK)|g' \ -e 's|@''HAVE_WCSSTR''@|$(HAVE_WCSSTR)|g' \ -e 's|@''HAVE_WCSTOK''@|$(HAVE_WCSTOK)|g' \ -e 's|@''HAVE_WCSWIDTH''@|$(HAVE_WCSWIDTH)|g' \ -e 's|@''HAVE_WCSFTIME''@|$(HAVE_WCSFTIME)|g' \ -e 's|@''HAVE_DECL_WCTOB''@|$(HAVE_DECL_WCTOB)|g' \ -e 's|@''HAVE_DECL_WCWIDTH''@|$(HAVE_DECL_WCWIDTH)|g' \ | \ sed -e 's|@''REPLACE_MBSTATE_T''@|$(REPLACE_MBSTATE_T)|g' \ -e 's|@''REPLACE_BTOWC''@|$(REPLACE_BTOWC)|g' \ -e 's|@''REPLACE_WCTOB''@|$(REPLACE_WCTOB)|g' \ -e 's|@''REPLACE_MBSINIT''@|$(REPLACE_MBSINIT)|g' \ -e 's|@''REPLACE_MBRTOWC''@|$(REPLACE_MBRTOWC)|g' \ -e 's|@''REPLACE_MBRLEN''@|$(REPLACE_MBRLEN)|g' \ -e 's|@''REPLACE_MBSRTOWCS''@|$(REPLACE_MBSRTOWCS)|g' \ -e 's|@''REPLACE_MBSNRTOWCS''@|$(REPLACE_MBSNRTOWCS)|g' \ -e 's|@''REPLACE_WCRTOMB''@|$(REPLACE_WCRTOMB)|g' \ -e 's|@''REPLACE_WCSRTOMBS''@|$(REPLACE_WCSRTOMBS)|g' \ -e 's|@''REPLACE_WCSNRTOMBS''@|$(REPLACE_WCSNRTOMBS)|g' \ -e 's|@''REPLACE_WCWIDTH''@|$(REPLACE_WCWIDTH)|g' \ -e 's|@''REPLACE_WCSWIDTH''@|$(REPLACE_WCSWIDTH)|g' \ -e 's|@''REPLACE_WCSFTIME''@|$(REPLACE_WCSFTIME)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ # We need the following in order to create when the system # doesn't have one that works with the given compiler. wctype.h: wctype.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_WCTYPE_H''@/$(HAVE_WCTYPE_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_WCTYPE_H''@|$(NEXT_WCTYPE_H)|g' \ -e 's/@''HAVE_CRTDEFS_H''@/$(HAVE_CRTDEFS_H)/g' \ -e 's/@''GNULIB_OVERRIDES_WINT_T''@/$(GNULIB_OVERRIDES_WINT_T)/g' \ -e 's/@''GNULIB_ISWBLANK''@/$(GNULIB_ISWBLANK)/g' \ -e 's/@''GNULIB_WCTYPE''@/$(GNULIB_WCTYPE)/g' \ -e 's/@''GNULIB_ISWCTYPE''@/$(GNULIB_ISWCTYPE)/g' \ -e 's/@''GNULIB_WCTRANS''@/$(GNULIB_WCTRANS)/g' \ -e 's/@''GNULIB_TOWCTRANS''@/$(GNULIB_TOWCTRANS)/g' \ -e 's/@''HAVE_ISWBLANK''@/$(HAVE_ISWBLANK)/g' \ -e 's/@''HAVE_ISWCNTRL''@/$(HAVE_ISWCNTRL)/g' \ -e 's/@''HAVE_WCTYPE_T''@/$(HAVE_WCTYPE_T)/g' \ -e 's/@''HAVE_WCTRANS_T''@/$(HAVE_WCTRANS_T)/g' \ -e 's/@''HAVE_WINT_T''@/$(HAVE_WINT_T)/g' \ -e 's/@''REPLACE_ISWBLANK''@/$(REPLACE_ISWBLANK)/g' \ -e 's/@''REPLACE_ISWCNTRL''@/$(REPLACE_ISWCNTRL)/g' \ -e 's/@''REPLACE_TOWLOWER''@/$(REPLACE_TOWLOWER)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/wctype.in.h; \ } > $@-t && \ mv $@-t $@ mostlyclean-local: mostlyclean-generic @for dir in '' $(MOSTLYCLEANDIRS); do \ if test -n "$$dir" && test -d $$dir; then \ echo "rmdir $$dir"; rmdir $$dir; \ fi; \ done; \ : # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: gnuastro-0.5/bootstrapped/lib/Makefile.am0000644000175000017500000024761413217200033015456 00000000000000## DO NOT EDIT! GENERATED AUTOMATICALLY! ## Process this file with automake to produce Makefile.in. # Copyright (C) 2002-2017 Free Software Foundation, Inc. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This file is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this file. If not, see . # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. # Reproduce by: gnulib-tool --import --local-dir=gl --lib=libgnu --source-base=bootstrapped/lib --m4-base=bootstrapped/m4 --doc-base=bootstrapped/doc --tests-base=bootstrapped/tests --aux-dir=bootstrapped/build-aux --with-tests --no-conditional-dependencies --libtool --macro-prefix=gl --no-vc-files argp error fdl func gendocs getline git-version-gen inttypes math mbstok_r nproc regex stdint strcase strtod AUTOMAKE_OPTIONS = 1.9.6 gnits subdir-objects SUBDIRS = noinst_HEADERS = noinst_LIBRARIES = noinst_LTLIBRARIES = EXTRA_DIST = BUILT_SOURCES = SUFFIXES = MOSTLYCLEANFILES = core *.stackdump MOSTLYCLEANDIRS = CLEANFILES = DISTCLEANFILES = MAINTAINERCLEANFILES = # No GNU Make output. AM_CPPFLAGS = AM_CFLAGS = noinst_LTLIBRARIES += libgnu.la libgnu_la_SOURCES = libgnu_la_LIBADD = $(gl_LTLIBOBJS) libgnu_la_DEPENDENCIES = $(gl_LTLIBOBJS) EXTRA_libgnu_la_SOURCES = libgnu_la_LDFLAGS = $(AM_LDFLAGS) libgnu_la_LDFLAGS += -no-undefined libgnu_la_LDFLAGS += $(LTLIBINTL) libgnu_la_LDFLAGS += $(LTLIBTHREAD) ## begin gnulib module absolute-header # Use this preprocessor expression to decide whether #include_next works. # Do not rely on a 'configure'-time test for this, since the expression # might appear in an installed header, which is used by some other compiler. HAVE_INCLUDE_NEXT = (__GNUC__ || 60000000 <= __DECC_VER) ## end gnulib module absolute-header ## begin gnulib module alloca libgnu_la_LIBADD += @LTALLOCA@ libgnu_la_DEPENDENCIES += @LTALLOCA@ EXTRA_DIST += alloca.c EXTRA_libgnu_la_SOURCES += alloca.c ## end gnulib module alloca ## begin gnulib module alloca-opt BUILT_SOURCES += $(ALLOCA_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_ALLOCA_H alloca.h: alloca.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/alloca.in.h; \ } > $@-t && \ mv -f $@-t $@ else alloca.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += alloca.h alloca.h-t EXTRA_DIST += alloca.in.h ## end gnulib module alloca-opt ## begin gnulib module argp libgnu_la_SOURCES += argp.h argp-ba.c argp-eexst.c argp-fmtstream.c argp-fmtstream.h argp-fs-xinl.c argp-help.c argp-namefrob.h argp-parse.c argp-pin.c argp-pv.c argp-pvh.c argp-xinl.c ## end gnulib module argp ## begin gnulib module btowc EXTRA_DIST += btowc.c EXTRA_libgnu_la_SOURCES += btowc.c ## end gnulib module btowc ## begin gnulib module c-ctype libgnu_la_SOURCES += c-ctype.h c-ctype.c ## end gnulib module c-ctype ## begin gnulib module configmake # Listed in the same order as the GNU makefile conventions, and # provided by autoconf 2.59c+ or 2.70. # The Automake-defined pkg* macros are appended, in the order # listed in the Automake 1.10a+ documentation. configmake.h: Makefile $(AM_V_GEN)rm -f $@-t && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ echo '#define PREFIX "$(prefix)"'; \ echo '#define EXEC_PREFIX "$(exec_prefix)"'; \ echo '#define BINDIR "$(bindir)"'; \ echo '#define SBINDIR "$(sbindir)"'; \ echo '#define LIBEXECDIR "$(libexecdir)"'; \ echo '#define DATAROOTDIR "$(datarootdir)"'; \ echo '#define DATADIR "$(datadir)"'; \ echo '#define SYSCONFDIR "$(sysconfdir)"'; \ echo '#define SHAREDSTATEDIR "$(sharedstatedir)"'; \ echo '#define LOCALSTATEDIR "$(localstatedir)"'; \ echo '#define RUNSTATEDIR "$(runstatedir)"'; \ echo '#define INCLUDEDIR "$(includedir)"'; \ echo '#define OLDINCLUDEDIR "$(oldincludedir)"'; \ echo '#define DOCDIR "$(docdir)"'; \ echo '#define INFODIR "$(infodir)"'; \ echo '#define HTMLDIR "$(htmldir)"'; \ echo '#define DVIDIR "$(dvidir)"'; \ echo '#define PDFDIR "$(pdfdir)"'; \ echo '#define PSDIR "$(psdir)"'; \ echo '#define LIBDIR "$(libdir)"'; \ echo '#define LISPDIR "$(lispdir)"'; \ echo '#define LOCALEDIR "$(localedir)"'; \ echo '#define MANDIR "$(mandir)"'; \ echo '#define MANEXT "$(manext)"'; \ echo '#define PKGDATADIR "$(pkgdatadir)"'; \ echo '#define PKGINCLUDEDIR "$(pkgincludedir)"'; \ echo '#define PKGLIBDIR "$(pkglibdir)"'; \ echo '#define PKGLIBEXECDIR "$(pkglibexecdir)"'; \ } | sed '/""/d' > $@-t && \ mv -f $@-t $@ BUILT_SOURCES += configmake.h CLEANFILES += configmake.h configmake.h-t ## end gnulib module configmake ## begin gnulib module dirname-lgpl libgnu_la_SOURCES += dirname-lgpl.c basename-lgpl.c stripslash.c EXTRA_DIST += dirname.h ## end gnulib module dirname-lgpl ## begin gnulib module dosname EXTRA_DIST += dosname.h ## end gnulib module dosname ## begin gnulib module errno BUILT_SOURCES += $(ERRNO_H) # We need the following in order to create when the system # doesn't have one that is POSIX compliant. if GL_GENERATE_ERRNO_H errno.h: errno.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_ERRNO_H''@|$(NEXT_ERRNO_H)|g' \ -e 's|@''EMULTIHOP_HIDDEN''@|$(EMULTIHOP_HIDDEN)|g' \ -e 's|@''EMULTIHOP_VALUE''@|$(EMULTIHOP_VALUE)|g' \ -e 's|@''ENOLINK_HIDDEN''@|$(ENOLINK_HIDDEN)|g' \ -e 's|@''ENOLINK_VALUE''@|$(ENOLINK_VALUE)|g' \ -e 's|@''EOVERFLOW_HIDDEN''@|$(EOVERFLOW_HIDDEN)|g' \ -e 's|@''EOVERFLOW_VALUE''@|$(EOVERFLOW_VALUE)|g' \ < $(srcdir)/errno.in.h; \ } > $@-t && \ mv $@-t $@ else errno.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += errno.h errno.h-t EXTRA_DIST += errno.in.h ## end gnulib module errno ## begin gnulib module error EXTRA_DIST += error.c error.h EXTRA_libgnu_la_SOURCES += error.c ## end gnulib module error ## begin gnulib module float BUILT_SOURCES += $(FLOAT_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_FLOAT_H float.h: float.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_FLOAT_H''@|$(NEXT_FLOAT_H)|g' \ -e 's|@''REPLACE_ITOLD''@|$(REPLACE_ITOLD)|g' \ < $(srcdir)/float.in.h; \ } > $@-t && \ mv $@-t $@ else float.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += float.h float.h-t EXTRA_DIST += float.c float.in.h itold.c EXTRA_libgnu_la_SOURCES += float.c itold.c ## end gnulib module float ## begin gnulib module gendocs EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/gendocs.sh ## end gnulib module gendocs ## begin gnulib module getdelim EXTRA_DIST += getdelim.c EXTRA_libgnu_la_SOURCES += getdelim.c ## end gnulib module getdelim ## begin gnulib module getline EXTRA_DIST += getline.c EXTRA_libgnu_la_SOURCES += getline.c ## end gnulib module getline ## begin gnulib module getopt-posix BUILT_SOURCES += $(GETOPT_H) $(GETOPT_CDEFS_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. getopt.h: getopt.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_GETOPT_H''@|$(HAVE_GETOPT_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_GETOPT_H''@|$(NEXT_GETOPT_H)|g' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ < $(srcdir)/getopt.in.h; \ } > $@-t && \ mv -f $@-t $@ getopt-cdefs.h: getopt-cdefs.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''HAVE_SYS_CDEFS_H''@|$(HAVE_SYS_CDEFS_H)|g' \ < $(srcdir)/getopt-cdefs.in.h; \ } > $@-t && \ mv -f $@-t $@ MOSTLYCLEANFILES += getopt.h getopt.h-t getopt-cdefs.h getopt-cdefs.h-t EXTRA_DIST += getopt-cdefs.in.h getopt-core.h getopt-ext.h getopt-pfx-core.h getopt-pfx-ext.h getopt.c getopt.in.h getopt1.c getopt_int.h EXTRA_libgnu_la_SOURCES += getopt.c getopt1.c ## end gnulib module getopt-posix ## begin gnulib module getprogname libgnu_la_SOURCES += getprogname.h getprogname.c ## end gnulib module getprogname ## begin gnulib module gettext-h libgnu_la_SOURCES += gettext.h ## end gnulib module gettext-h ## begin gnulib module git-version-gen EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/git-version-gen ## end gnulib module git-version-gen ## begin gnulib module hard-locale libgnu_la_SOURCES += hard-locale.c EXTRA_DIST += hard-locale.h ## end gnulib module hard-locale ## begin gnulib module havelib EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/config.rpath ## end gnulib module havelib ## begin gnulib module intprops EXTRA_DIST += intprops.h ## end gnulib module intprops ## begin gnulib module inttypes-incomplete BUILT_SOURCES += inttypes.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. inttypes.h: inttypes.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's/@''HAVE_INTTYPES_H''@/$(HAVE_INTTYPES_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_INTTYPES_H''@|$(NEXT_INTTYPES_H)|g' \ -e 's/@''PRI_MACROS_BROKEN''@/$(PRI_MACROS_BROKEN)/g' \ -e 's/@''APPLE_UNIVERSAL_BUILD''@/$(APPLE_UNIVERSAL_BUILD)/g' \ -e 's/@''HAVE_LONG_LONG_INT''@/$(HAVE_LONG_LONG_INT)/g' \ -e 's/@''HAVE_UNSIGNED_LONG_LONG_INT''@/$(HAVE_UNSIGNED_LONG_LONG_INT)/g' \ -e 's/@''PRIPTR_PREFIX''@/$(PRIPTR_PREFIX)/g' \ -e 's/@''GNULIB_IMAXABS''@/$(GNULIB_IMAXABS)/g' \ -e 's/@''GNULIB_IMAXDIV''@/$(GNULIB_IMAXDIV)/g' \ -e 's/@''GNULIB_STRTOIMAX''@/$(GNULIB_STRTOIMAX)/g' \ -e 's/@''GNULIB_STRTOUMAX''@/$(GNULIB_STRTOUMAX)/g' \ -e 's/@''HAVE_DECL_IMAXABS''@/$(HAVE_DECL_IMAXABS)/g' \ -e 's/@''HAVE_DECL_IMAXDIV''@/$(HAVE_DECL_IMAXDIV)/g' \ -e 's/@''HAVE_DECL_STRTOIMAX''@/$(HAVE_DECL_STRTOIMAX)/g' \ -e 's/@''HAVE_DECL_STRTOUMAX''@/$(HAVE_DECL_STRTOUMAX)/g' \ -e 's/@''REPLACE_STRTOIMAX''@/$(REPLACE_STRTOIMAX)/g' \ -e 's/@''REPLACE_STRTOUMAX''@/$(REPLACE_STRTOUMAX)/g' \ -e 's/@''INT32_MAX_LT_INTMAX_MAX''@/$(INT32_MAX_LT_INTMAX_MAX)/g' \ -e 's/@''INT64_MAX_EQ_LONG_MAX''@/$(INT64_MAX_EQ_LONG_MAX)/g' \ -e 's/@''UINT32_MAX_LT_UINTMAX_MAX''@/$(UINT32_MAX_LT_UINTMAX_MAX)/g' \ -e 's/@''UINT64_MAX_EQ_ULONG_MAX''@/$(UINT64_MAX_EQ_ULONG_MAX)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/inttypes.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += inttypes.h inttypes.h-t EXTRA_DIST += inttypes.in.h ## end gnulib module inttypes-incomplete ## begin gnulib module iswblank EXTRA_DIST += iswblank.c EXTRA_libgnu_la_SOURCES += iswblank.c ## end gnulib module iswblank ## begin gnulib module langinfo BUILT_SOURCES += langinfo.h # We need the following in order to create an empty placeholder for # when the system doesn't have one. langinfo.h: langinfo.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_LANGINFO_H''@|$(HAVE_LANGINFO_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_LANGINFO_H''@|$(NEXT_LANGINFO_H)|g' \ -e 's/@''GNULIB_NL_LANGINFO''@/$(GNULIB_NL_LANGINFO)/g' \ -e 's|@''HAVE_LANGINFO_CODESET''@|$(HAVE_LANGINFO_CODESET)|g' \ -e 's|@''HAVE_LANGINFO_T_FMT_AMPM''@|$(HAVE_LANGINFO_T_FMT_AMPM)|g' \ -e 's|@''HAVE_LANGINFO_ERA''@|$(HAVE_LANGINFO_ERA)|g' \ -e 's|@''HAVE_LANGINFO_YESEXPR''@|$(HAVE_LANGINFO_YESEXPR)|g' \ -e 's|@''HAVE_NL_LANGINFO''@|$(HAVE_NL_LANGINFO)|g' \ -e 's|@''REPLACE_NL_LANGINFO''@|$(REPLACE_NL_LANGINFO)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/langinfo.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += langinfo.h langinfo.h-t EXTRA_DIST += langinfo.in.h ## end gnulib module langinfo ## begin gnulib module limits-h BUILT_SOURCES += $(LIMITS_H) # We need the following in order to create when the system # doesn't have one that is compatible with GNU. if GL_GENERATE_LIMITS_H limits.h: limits.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_LIMITS_H''@|$(NEXT_LIMITS_H)|g' \ < $(srcdir)/limits.in.h; \ } > $@-t && \ mv $@-t $@ else limits.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += limits.h limits.h-t EXTRA_DIST += limits.in.h ## end gnulib module limits-h ## begin gnulib module localcharset libgnu_la_SOURCES += localcharset.h localcharset.c # We need the following in order to install a simple file in $(libdir) # which is shared with other installed packages. We use a list of referencing # packages so that "make uninstall" will remove the file if and only if it # is not used by another installed package. # On systems with glibc-2.1 or newer, the file is redundant, therefore we # avoid installing it. all-local: charset.alias ref-add.sed ref-del.sed charset_alias = $(DESTDIR)$(libdir)/charset.alias charset_tmp = $(DESTDIR)$(libdir)/charset.tmp install-exec-local: install-exec-localcharset install-exec-localcharset: all-local if test $(GLIBC21) = no; then \ case '$(host_os)' in \ darwin[56]*) \ need_charset_alias=true ;; \ darwin* | cygwin* | mingw* | pw32* | cegcc*) \ need_charset_alias=false ;; \ *) \ need_charset_alias=true ;; \ esac ; \ else \ need_charset_alias=false ; \ fi ; \ if $$need_charset_alias; then \ $(mkinstalldirs) $(DESTDIR)$(libdir) ; \ fi ; \ if test -f $(charset_alias); then \ sed -f ref-add.sed $(charset_alias) > $(charset_tmp) ; \ $(INSTALL_DATA) $(charset_tmp) $(charset_alias) ; \ rm -f $(charset_tmp) ; \ else \ if $$need_charset_alias; then \ sed -f ref-add.sed charset.alias > $(charset_tmp) ; \ $(INSTALL_DATA) $(charset_tmp) $(charset_alias) ; \ rm -f $(charset_tmp) ; \ fi ; \ fi uninstall-local: uninstall-localcharset uninstall-localcharset: all-local if test -f $(charset_alias); then \ sed -f ref-del.sed $(charset_alias) > $(charset_tmp); \ if grep '^# Packages using this file: $$' $(charset_tmp) \ > /dev/null; then \ rm -f $(charset_alias); \ else \ $(INSTALL_DATA) $(charset_tmp) $(charset_alias); \ fi; \ rm -f $(charset_tmp); \ fi charset.alias: config.charset $(AM_V_GEN)rm -f t-$@ $@ && \ $(SHELL) $(srcdir)/config.charset '$(host)' > t-$@ && \ mv t-$@ $@ SUFFIXES += .sed .sin .sin.sed: $(AM_V_GEN)rm -f t-$@ $@ && \ sed -e '/^#/d' -e 's/@''PACKAGE''@/$(PACKAGE)/g' $< > t-$@ && \ mv t-$@ $@ CLEANFILES += charset.alias ref-add.sed ref-del.sed EXTRA_DIST += config.charset ref-add.sin ref-del.sin ## end gnulib module localcharset ## begin gnulib module locale BUILT_SOURCES += locale.h # We need the following in order to create when the system # doesn't have one that provides all definitions. locale.h: locale.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_LOCALE_H''@|$(NEXT_LOCALE_H)|g' \ -e 's/@''GNULIB_LOCALECONV''@/$(GNULIB_LOCALECONV)/g' \ -e 's/@''GNULIB_SETLOCALE''@/$(GNULIB_SETLOCALE)/g' \ -e 's/@''GNULIB_DUPLOCALE''@/$(GNULIB_DUPLOCALE)/g' \ -e 's|@''HAVE_DUPLOCALE''@|$(HAVE_DUPLOCALE)|g' \ -e 's|@''HAVE_XLOCALE_H''@|$(HAVE_XLOCALE_H)|g' \ -e 's|@''REPLACE_LOCALECONV''@|$(REPLACE_LOCALECONV)|g' \ -e 's|@''REPLACE_SETLOCALE''@|$(REPLACE_SETLOCALE)|g' \ -e 's|@''REPLACE_DUPLOCALE''@|$(REPLACE_DUPLOCALE)|g' \ -e 's|@''REPLACE_STRUCT_LCONV''@|$(REPLACE_STRUCT_LCONV)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/locale.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += locale.h locale.h-t EXTRA_DIST += locale.in.h ## end gnulib module locale ## begin gnulib module localeconv EXTRA_DIST += localeconv.c EXTRA_libgnu_la_SOURCES += localeconv.c ## end gnulib module localeconv ## begin gnulib module lock libgnu_la_SOURCES += glthread/lock.h glthread/lock.c ## end gnulib module lock ## begin gnulib module malloc-gnu EXTRA_DIST += malloc.c EXTRA_libgnu_la_SOURCES += malloc.c ## end gnulib module malloc-gnu ## begin gnulib module malloc-posix EXTRA_DIST += malloc.c EXTRA_libgnu_la_SOURCES += malloc.c ## end gnulib module malloc-posix ## begin gnulib module math BUILT_SOURCES += math.h libgnu_la_SOURCES += math.c # We need the following in order to create when the system # doesn't have one that works with the given compiler. math.h: math.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT_AS_FIRST_DIRECTIVE''@|$(INCLUDE_NEXT_AS_FIRST_DIRECTIVE)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_AS_FIRST_DIRECTIVE_MATH_H''@|$(NEXT_AS_FIRST_DIRECTIVE_MATH_H)|g' \ -e 's/@''GNULIB_ACOSF''@/$(GNULIB_ACOSF)/g' \ -e 's/@''GNULIB_ACOSL''@/$(GNULIB_ACOSL)/g' \ -e 's/@''GNULIB_ASINF''@/$(GNULIB_ASINF)/g' \ -e 's/@''GNULIB_ASINL''@/$(GNULIB_ASINL)/g' \ -e 's/@''GNULIB_ATANF''@/$(GNULIB_ATANF)/g' \ -e 's/@''GNULIB_ATANL''@/$(GNULIB_ATANL)/g' \ -e 's/@''GNULIB_ATAN2F''@/$(GNULIB_ATAN2F)/g' \ -e 's/@''GNULIB_CBRT''@/$(GNULIB_CBRT)/g' \ -e 's/@''GNULIB_CBRTF''@/$(GNULIB_CBRTF)/g' \ -e 's/@''GNULIB_CBRTL''@/$(GNULIB_CBRTL)/g' \ -e 's/@''GNULIB_CEIL''@/$(GNULIB_CEIL)/g' \ -e 's/@''GNULIB_CEILF''@/$(GNULIB_CEILF)/g' \ -e 's/@''GNULIB_CEILL''@/$(GNULIB_CEILL)/g' \ -e 's/@''GNULIB_COPYSIGN''@/$(GNULIB_COPYSIGN)/g' \ -e 's/@''GNULIB_COPYSIGNF''@/$(GNULIB_COPYSIGNF)/g' \ -e 's/@''GNULIB_COPYSIGNL''@/$(GNULIB_COPYSIGNL)/g' \ -e 's/@''GNULIB_COSF''@/$(GNULIB_COSF)/g' \ -e 's/@''GNULIB_COSL''@/$(GNULIB_COSL)/g' \ -e 's/@''GNULIB_COSHF''@/$(GNULIB_COSHF)/g' \ -e 's/@''GNULIB_EXPF''@/$(GNULIB_EXPF)/g' \ -e 's/@''GNULIB_EXPL''@/$(GNULIB_EXPL)/g' \ -e 's/@''GNULIB_EXP2''@/$(GNULIB_EXP2)/g' \ -e 's/@''GNULIB_EXP2F''@/$(GNULIB_EXP2F)/g' \ -e 's/@''GNULIB_EXP2L''@/$(GNULIB_EXP2L)/g' \ -e 's/@''GNULIB_EXPM1''@/$(GNULIB_EXPM1)/g' \ -e 's/@''GNULIB_EXPM1F''@/$(GNULIB_EXPM1F)/g' \ -e 's/@''GNULIB_EXPM1L''@/$(GNULIB_EXPM1L)/g' \ -e 's/@''GNULIB_FABSF''@/$(GNULIB_FABSF)/g' \ -e 's/@''GNULIB_FABSL''@/$(GNULIB_FABSL)/g' \ -e 's/@''GNULIB_FLOOR''@/$(GNULIB_FLOOR)/g' \ -e 's/@''GNULIB_FLOORF''@/$(GNULIB_FLOORF)/g' \ -e 's/@''GNULIB_FLOORL''@/$(GNULIB_FLOORL)/g' \ -e 's/@''GNULIB_FMA''@/$(GNULIB_FMA)/g' \ -e 's/@''GNULIB_FMAF''@/$(GNULIB_FMAF)/g' \ -e 's/@''GNULIB_FMAL''@/$(GNULIB_FMAL)/g' \ -e 's/@''GNULIB_FMOD''@/$(GNULIB_FMOD)/g' \ -e 's/@''GNULIB_FMODF''@/$(GNULIB_FMODF)/g' \ -e 's/@''GNULIB_FMODL''@/$(GNULIB_FMODL)/g' \ -e 's/@''GNULIB_FREXPF''@/$(GNULIB_FREXPF)/g' \ -e 's/@''GNULIB_FREXP''@/$(GNULIB_FREXP)/g' \ -e 's/@''GNULIB_FREXPL''@/$(GNULIB_FREXPL)/g' \ -e 's/@''GNULIB_HYPOT''@/$(GNULIB_HYPOT)/g' \ -e 's/@''GNULIB_HYPOTF''@/$(GNULIB_HYPOTF)/g' \ -e 's/@''GNULIB_HYPOTL''@/$(GNULIB_HYPOTL)/g' \ < $(srcdir)/math.in.h | \ sed -e 's/@''GNULIB_ILOGB''@/$(GNULIB_ILOGB)/g' \ -e 's/@''GNULIB_ILOGBF''@/$(GNULIB_ILOGBF)/g' \ -e 's/@''GNULIB_ILOGBL''@/$(GNULIB_ILOGBL)/g' \ -e 's/@''GNULIB_ISFINITE''@/$(GNULIB_ISFINITE)/g' \ -e 's/@''GNULIB_ISINF''@/$(GNULIB_ISINF)/g' \ -e 's/@''GNULIB_ISNAN''@/$(GNULIB_ISNAN)/g' \ -e 's/@''GNULIB_ISNANF''@/$(GNULIB_ISNANF)/g' \ -e 's/@''GNULIB_ISNAND''@/$(GNULIB_ISNAND)/g' \ -e 's/@''GNULIB_ISNANL''@/$(GNULIB_ISNANL)/g' \ -e 's/@''GNULIB_LDEXPF''@/$(GNULIB_LDEXPF)/g' \ -e 's/@''GNULIB_LDEXPL''@/$(GNULIB_LDEXPL)/g' \ -e 's/@''GNULIB_LOG''@/$(GNULIB_LOG)/g' \ -e 's/@''GNULIB_LOGF''@/$(GNULIB_LOGF)/g' \ -e 's/@''GNULIB_LOGL''@/$(GNULIB_LOGL)/g' \ -e 's/@''GNULIB_LOG10''@/$(GNULIB_LOG10)/g' \ -e 's/@''GNULIB_LOG10F''@/$(GNULIB_LOG10F)/g' \ -e 's/@''GNULIB_LOG10L''@/$(GNULIB_LOG10L)/g' \ -e 's/@''GNULIB_LOG1P''@/$(GNULIB_LOG1P)/g' \ -e 's/@''GNULIB_LOG1PF''@/$(GNULIB_LOG1PF)/g' \ -e 's/@''GNULIB_LOG1PL''@/$(GNULIB_LOG1PL)/g' \ -e 's/@''GNULIB_LOG2''@/$(GNULIB_LOG2)/g' \ -e 's/@''GNULIB_LOG2F''@/$(GNULIB_LOG2F)/g' \ -e 's/@''GNULIB_LOG2L''@/$(GNULIB_LOG2L)/g' \ -e 's/@''GNULIB_LOGB''@/$(GNULIB_LOGB)/g' \ -e 's/@''GNULIB_LOGBF''@/$(GNULIB_LOGBF)/g' \ -e 's/@''GNULIB_LOGBL''@/$(GNULIB_LOGBL)/g' \ -e 's/@''GNULIB_MODF''@/$(GNULIB_MODF)/g' \ -e 's/@''GNULIB_MODFF''@/$(GNULIB_MODFF)/g' \ -e 's/@''GNULIB_MODFL''@/$(GNULIB_MODFL)/g' \ -e 's/@''GNULIB_POWF''@/$(GNULIB_POWF)/g' \ -e 's/@''GNULIB_REMAINDER''@/$(GNULIB_REMAINDER)/g' \ -e 's/@''GNULIB_REMAINDERF''@/$(GNULIB_REMAINDERF)/g' \ -e 's/@''GNULIB_REMAINDERL''@/$(GNULIB_REMAINDERL)/g' \ -e 's/@''GNULIB_RINT''@/$(GNULIB_RINT)/g' \ -e 's/@''GNULIB_RINTF''@/$(GNULIB_RINTF)/g' \ -e 's/@''GNULIB_RINTL''@/$(GNULIB_RINTL)/g' \ -e 's/@''GNULIB_ROUND''@/$(GNULIB_ROUND)/g' \ -e 's/@''GNULIB_ROUNDF''@/$(GNULIB_ROUNDF)/g' \ -e 's/@''GNULIB_ROUNDL''@/$(GNULIB_ROUNDL)/g' \ -e 's/@''GNULIB_SIGNBIT''@/$(GNULIB_SIGNBIT)/g' \ -e 's/@''GNULIB_SINF''@/$(GNULIB_SINF)/g' \ -e 's/@''GNULIB_SINL''@/$(GNULIB_SINL)/g' \ -e 's/@''GNULIB_SINHF''@/$(GNULIB_SINHF)/g' \ -e 's/@''GNULIB_SQRTF''@/$(GNULIB_SQRTF)/g' \ -e 's/@''GNULIB_SQRTL''@/$(GNULIB_SQRTL)/g' \ -e 's/@''GNULIB_TANF''@/$(GNULIB_TANF)/g' \ -e 's/@''GNULIB_TANL''@/$(GNULIB_TANL)/g' \ -e 's/@''GNULIB_TANHF''@/$(GNULIB_TANHF)/g' \ -e 's/@''GNULIB_TRUNC''@/$(GNULIB_TRUNC)/g' \ -e 's/@''GNULIB_TRUNCF''@/$(GNULIB_TRUNCF)/g' \ -e 's/@''GNULIB_TRUNCL''@/$(GNULIB_TRUNCL)/g' \ | \ sed -e 's|@''HAVE_ACOSF''@|$(HAVE_ACOSF)|g' \ -e 's|@''HAVE_ACOSL''@|$(HAVE_ACOSL)|g' \ -e 's|@''HAVE_ASINF''@|$(HAVE_ASINF)|g' \ -e 's|@''HAVE_ASINL''@|$(HAVE_ASINL)|g' \ -e 's|@''HAVE_ATANF''@|$(HAVE_ATANF)|g' \ -e 's|@''HAVE_ATANL''@|$(HAVE_ATANL)|g' \ -e 's|@''HAVE_ATAN2F''@|$(HAVE_ATAN2F)|g' \ -e 's|@''HAVE_CBRT''@|$(HAVE_CBRT)|g' \ -e 's|@''HAVE_CBRTF''@|$(HAVE_CBRTF)|g' \ -e 's|@''HAVE_CBRTL''@|$(HAVE_CBRTL)|g' \ -e 's|@''HAVE_COPYSIGN''@|$(HAVE_COPYSIGN)|g' \ -e 's|@''HAVE_COPYSIGNL''@|$(HAVE_COPYSIGNL)|g' \ -e 's|@''HAVE_COSF''@|$(HAVE_COSF)|g' \ -e 's|@''HAVE_COSL''@|$(HAVE_COSL)|g' \ -e 's|@''HAVE_COSHF''@|$(HAVE_COSHF)|g' \ -e 's|@''HAVE_EXPF''@|$(HAVE_EXPF)|g' \ -e 's|@''HAVE_EXPL''@|$(HAVE_EXPL)|g' \ -e 's|@''HAVE_EXPM1''@|$(HAVE_EXPM1)|g' \ -e 's|@''HAVE_EXPM1F''@|$(HAVE_EXPM1F)|g' \ -e 's|@''HAVE_FABSF''@|$(HAVE_FABSF)|g' \ -e 's|@''HAVE_FABSL''@|$(HAVE_FABSL)|g' \ -e 's|@''HAVE_FMA''@|$(HAVE_FMA)|g' \ -e 's|@''HAVE_FMAF''@|$(HAVE_FMAF)|g' \ -e 's|@''HAVE_FMAL''@|$(HAVE_FMAL)|g' \ -e 's|@''HAVE_FMODF''@|$(HAVE_FMODF)|g' \ -e 's|@''HAVE_FMODL''@|$(HAVE_FMODL)|g' \ -e 's|@''HAVE_FREXPF''@|$(HAVE_FREXPF)|g' \ -e 's|@''HAVE_HYPOTF''@|$(HAVE_HYPOTF)|g' \ -e 's|@''HAVE_HYPOTL''@|$(HAVE_HYPOTL)|g' \ -e 's|@''HAVE_ILOGB''@|$(HAVE_ILOGB)|g' \ -e 's|@''HAVE_ILOGBF''@|$(HAVE_ILOGBF)|g' \ -e 's|@''HAVE_ILOGBL''@|$(HAVE_ILOGBL)|g' \ -e 's|@''HAVE_ISNANF''@|$(HAVE_ISNANF)|g' \ -e 's|@''HAVE_ISNAND''@|$(HAVE_ISNAND)|g' \ -e 's|@''HAVE_ISNANL''@|$(HAVE_ISNANL)|g' \ -e 's|@''HAVE_LDEXPF''@|$(HAVE_LDEXPF)|g' \ -e 's|@''HAVE_LOGF''@|$(HAVE_LOGF)|g' \ -e 's|@''HAVE_LOGL''@|$(HAVE_LOGL)|g' \ -e 's|@''HAVE_LOG10F''@|$(HAVE_LOG10F)|g' \ -e 's|@''HAVE_LOG10L''@|$(HAVE_LOG10L)|g' \ -e 's|@''HAVE_LOG1P''@|$(HAVE_LOG1P)|g' \ -e 's|@''HAVE_LOG1PF''@|$(HAVE_LOG1PF)|g' \ -e 's|@''HAVE_LOG1PL''@|$(HAVE_LOG1PL)|g' \ -e 's|@''HAVE_LOGBF''@|$(HAVE_LOGBF)|g' \ -e 's|@''HAVE_LOGBL''@|$(HAVE_LOGBL)|g' \ -e 's|@''HAVE_MODFF''@|$(HAVE_MODFF)|g' \ -e 's|@''HAVE_MODFL''@|$(HAVE_MODFL)|g' \ -e 's|@''HAVE_POWF''@|$(HAVE_POWF)|g' \ -e 's|@''HAVE_REMAINDER''@|$(HAVE_REMAINDER)|g' \ -e 's|@''HAVE_REMAINDERF''@|$(HAVE_REMAINDERF)|g' \ -e 's|@''HAVE_RINT''@|$(HAVE_RINT)|g' \ -e 's|@''HAVE_RINTL''@|$(HAVE_RINTL)|g' \ -e 's|@''HAVE_SINF''@|$(HAVE_SINF)|g' \ -e 's|@''HAVE_SINL''@|$(HAVE_SINL)|g' \ -e 's|@''HAVE_SINHF''@|$(HAVE_SINHF)|g' \ -e 's|@''HAVE_SQRTF''@|$(HAVE_SQRTF)|g' \ -e 's|@''HAVE_SQRTL''@|$(HAVE_SQRTL)|g' \ -e 's|@''HAVE_TANF''@|$(HAVE_TANF)|g' \ -e 's|@''HAVE_TANL''@|$(HAVE_TANL)|g' \ -e 's|@''HAVE_TANHF''@|$(HAVE_TANHF)|g' \ -e 's|@''HAVE_DECL_ACOSL''@|$(HAVE_DECL_ACOSL)|g' \ -e 's|@''HAVE_DECL_ASINL''@|$(HAVE_DECL_ASINL)|g' \ -e 's|@''HAVE_DECL_ATANL''@|$(HAVE_DECL_ATANL)|g' \ -e 's|@''HAVE_DECL_CBRTF''@|$(HAVE_DECL_CBRTF)|g' \ -e 's|@''HAVE_DECL_CBRTL''@|$(HAVE_DECL_CBRTL)|g' \ -e 's|@''HAVE_DECL_CEILF''@|$(HAVE_DECL_CEILF)|g' \ -e 's|@''HAVE_DECL_CEILL''@|$(HAVE_DECL_CEILL)|g' \ -e 's|@''HAVE_DECL_COPYSIGNF''@|$(HAVE_DECL_COPYSIGNF)|g' \ -e 's|@''HAVE_DECL_COSL''@|$(HAVE_DECL_COSL)|g' \ -e 's|@''HAVE_DECL_EXPL''@|$(HAVE_DECL_EXPL)|g' \ -e 's|@''HAVE_DECL_EXP2''@|$(HAVE_DECL_EXP2)|g' \ -e 's|@''HAVE_DECL_EXP2F''@|$(HAVE_DECL_EXP2F)|g' \ -e 's|@''HAVE_DECL_EXP2L''@|$(HAVE_DECL_EXP2L)|g' \ -e 's|@''HAVE_DECL_EXPM1L''@|$(HAVE_DECL_EXPM1L)|g' \ -e 's|@''HAVE_DECL_FLOORF''@|$(HAVE_DECL_FLOORF)|g' \ -e 's|@''HAVE_DECL_FLOORL''@|$(HAVE_DECL_FLOORL)|g' \ -e 's|@''HAVE_DECL_FREXPL''@|$(HAVE_DECL_FREXPL)|g' \ -e 's|@''HAVE_DECL_LDEXPL''@|$(HAVE_DECL_LDEXPL)|g' \ -e 's|@''HAVE_DECL_LOGL''@|$(HAVE_DECL_LOGL)|g' \ -e 's|@''HAVE_DECL_LOG10L''@|$(HAVE_DECL_LOG10L)|g' \ -e 's|@''HAVE_DECL_LOG2''@|$(HAVE_DECL_LOG2)|g' \ -e 's|@''HAVE_DECL_LOG2F''@|$(HAVE_DECL_LOG2F)|g' \ -e 's|@''HAVE_DECL_LOG2L''@|$(HAVE_DECL_LOG2L)|g' \ -e 's|@''HAVE_DECL_LOGB''@|$(HAVE_DECL_LOGB)|g' \ -e 's|@''HAVE_DECL_REMAINDER''@|$(HAVE_DECL_REMAINDER)|g' \ -e 's|@''HAVE_DECL_REMAINDERL''@|$(HAVE_DECL_REMAINDERL)|g' \ -e 's|@''HAVE_DECL_RINTF''@|$(HAVE_DECL_RINTF)|g' \ -e 's|@''HAVE_DECL_ROUND''@|$(HAVE_DECL_ROUND)|g' \ -e 's|@''HAVE_DECL_ROUNDF''@|$(HAVE_DECL_ROUNDF)|g' \ -e 's|@''HAVE_DECL_ROUNDL''@|$(HAVE_DECL_ROUNDL)|g' \ -e 's|@''HAVE_DECL_SINL''@|$(HAVE_DECL_SINL)|g' \ -e 's|@''HAVE_DECL_SQRTL''@|$(HAVE_DECL_SQRTL)|g' \ -e 's|@''HAVE_DECL_TANL''@|$(HAVE_DECL_TANL)|g' \ -e 's|@''HAVE_DECL_TRUNC''@|$(HAVE_DECL_TRUNC)|g' \ -e 's|@''HAVE_DECL_TRUNCF''@|$(HAVE_DECL_TRUNCF)|g' \ -e 's|@''HAVE_DECL_TRUNCL''@|$(HAVE_DECL_TRUNCL)|g' \ | \ sed -e 's|@''REPLACE_ACOSF''@|$(REPLACE_ACOSF)|g' \ -e 's|@''REPLACE_ASINF''@|$(REPLACE_ASINF)|g' \ -e 's|@''REPLACE_ATANF''@|$(REPLACE_ATANF)|g' \ -e 's|@''REPLACE_ATAN2F''@|$(REPLACE_ATAN2F)|g' \ -e 's|@''REPLACE_CBRTF''@|$(REPLACE_CBRTF)|g' \ -e 's|@''REPLACE_CBRTL''@|$(REPLACE_CBRTL)|g' \ -e 's|@''REPLACE_CEIL''@|$(REPLACE_CEIL)|g' \ -e 's|@''REPLACE_CEILF''@|$(REPLACE_CEILF)|g' \ -e 's|@''REPLACE_CEILL''@|$(REPLACE_CEILL)|g' \ -e 's|@''REPLACE_COSF''@|$(REPLACE_COSF)|g' \ -e 's|@''REPLACE_COSHF''@|$(REPLACE_COSHF)|g' \ -e 's|@''REPLACE_EXPF''@|$(REPLACE_EXPF)|g' \ -e 's|@''REPLACE_EXPM1''@|$(REPLACE_EXPM1)|g' \ -e 's|@''REPLACE_EXPM1F''@|$(REPLACE_EXPM1F)|g' \ -e 's|@''REPLACE_EXP2''@|$(REPLACE_EXP2)|g' \ -e 's|@''REPLACE_EXP2L''@|$(REPLACE_EXP2L)|g' \ -e 's|@''REPLACE_FABSL''@|$(REPLACE_FABSL)|g' \ -e 's|@''REPLACE_FLOOR''@|$(REPLACE_FLOOR)|g' \ -e 's|@''REPLACE_FLOORF''@|$(REPLACE_FLOORF)|g' \ -e 's|@''REPLACE_FLOORL''@|$(REPLACE_FLOORL)|g' \ -e 's|@''REPLACE_FMA''@|$(REPLACE_FMA)|g' \ -e 's|@''REPLACE_FMAF''@|$(REPLACE_FMAF)|g' \ -e 's|@''REPLACE_FMAL''@|$(REPLACE_FMAL)|g' \ -e 's|@''REPLACE_FMOD''@|$(REPLACE_FMOD)|g' \ -e 's|@''REPLACE_FMODF''@|$(REPLACE_FMODF)|g' \ -e 's|@''REPLACE_FMODL''@|$(REPLACE_FMODL)|g' \ -e 's|@''REPLACE_FREXPF''@|$(REPLACE_FREXPF)|g' \ -e 's|@''REPLACE_FREXP''@|$(REPLACE_FREXP)|g' \ -e 's|@''REPLACE_FREXPL''@|$(REPLACE_FREXPL)|g' \ -e 's|@''REPLACE_HUGE_VAL''@|$(REPLACE_HUGE_VAL)|g' \ -e 's|@''REPLACE_HYPOT''@|$(REPLACE_HYPOT)|g' \ -e 's|@''REPLACE_HYPOTF''@|$(REPLACE_HYPOTF)|g' \ -e 's|@''REPLACE_HYPOTL''@|$(REPLACE_HYPOTL)|g' \ -e 's|@''REPLACE_ILOGB''@|$(REPLACE_ILOGB)|g' \ -e 's|@''REPLACE_ILOGBF''@|$(REPLACE_ILOGBF)|g' \ -e 's|@''REPLACE_ILOGBL''@|$(REPLACE_ILOGBL)|g' \ -e 's|@''REPLACE_ISFINITE''@|$(REPLACE_ISFINITE)|g' \ -e 's|@''REPLACE_ISINF''@|$(REPLACE_ISINF)|g' \ -e 's|@''REPLACE_ISNAN''@|$(REPLACE_ISNAN)|g' \ -e 's|@''REPLACE_ITOLD''@|$(REPLACE_ITOLD)|g' \ -e 's|@''REPLACE_LDEXPL''@|$(REPLACE_LDEXPL)|g' \ -e 's|@''REPLACE_LOG''@|$(REPLACE_LOG)|g' \ -e 's|@''REPLACE_LOGF''@|$(REPLACE_LOGF)|g' \ -e 's|@''REPLACE_LOGL''@|$(REPLACE_LOGL)|g' \ -e 's|@''REPLACE_LOG10''@|$(REPLACE_LOG10)|g' \ -e 's|@''REPLACE_LOG10F''@|$(REPLACE_LOG10F)|g' \ -e 's|@''REPLACE_LOG10L''@|$(REPLACE_LOG10L)|g' \ -e 's|@''REPLACE_LOG1P''@|$(REPLACE_LOG1P)|g' \ -e 's|@''REPLACE_LOG1PF''@|$(REPLACE_LOG1PF)|g' \ -e 's|@''REPLACE_LOG1PL''@|$(REPLACE_LOG1PL)|g' \ -e 's|@''REPLACE_LOG2''@|$(REPLACE_LOG2)|g' \ -e 's|@''REPLACE_LOG2F''@|$(REPLACE_LOG2F)|g' \ -e 's|@''REPLACE_LOG2L''@|$(REPLACE_LOG2L)|g' \ -e 's|@''REPLACE_LOGB''@|$(REPLACE_LOGB)|g' \ -e 's|@''REPLACE_LOGBF''@|$(REPLACE_LOGBF)|g' \ -e 's|@''REPLACE_LOGBL''@|$(REPLACE_LOGBL)|g' \ -e 's|@''REPLACE_MODF''@|$(REPLACE_MODF)|g' \ -e 's|@''REPLACE_MODFF''@|$(REPLACE_MODFF)|g' \ -e 's|@''REPLACE_MODFL''@|$(REPLACE_MODFL)|g' \ -e 's|@''REPLACE_NAN''@|$(REPLACE_NAN)|g' \ -e 's|@''REPLACE_REMAINDER''@|$(REPLACE_REMAINDER)|g' \ -e 's|@''REPLACE_REMAINDERF''@|$(REPLACE_REMAINDERF)|g' \ -e 's|@''REPLACE_REMAINDERL''@|$(REPLACE_REMAINDERL)|g' \ -e 's|@''REPLACE_ROUND''@|$(REPLACE_ROUND)|g' \ -e 's|@''REPLACE_ROUNDF''@|$(REPLACE_ROUNDF)|g' \ -e 's|@''REPLACE_ROUNDL''@|$(REPLACE_ROUNDL)|g' \ -e 's|@''REPLACE_SIGNBIT''@|$(REPLACE_SIGNBIT)|g' \ -e 's|@''REPLACE_SIGNBIT_USING_GCC''@|$(REPLACE_SIGNBIT_USING_GCC)|g' \ -e 's|@''REPLACE_SINF''@|$(REPLACE_SINF)|g' \ -e 's|@''REPLACE_SINHF''@|$(REPLACE_SINHF)|g' \ -e 's|@''REPLACE_SQRTF''@|$(REPLACE_SQRTF)|g' \ -e 's|@''REPLACE_SQRTL''@|$(REPLACE_SQRTL)|g' \ -e 's|@''REPLACE_TANF''@|$(REPLACE_TANF)|g' \ -e 's|@''REPLACE_TANHF''@|$(REPLACE_TANHF)|g' \ -e 's|@''REPLACE_TRUNC''@|$(REPLACE_TRUNC)|g' \ -e 's|@''REPLACE_TRUNCF''@|$(REPLACE_TRUNCF)|g' \ -e 's|@''REPLACE_TRUNCL''@|$(REPLACE_TRUNCL)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += math.h math.h-t EXTRA_DIST += math.in.h ## end gnulib module math ## begin gnulib module mbchar libgnu_la_SOURCES += mbchar.c EXTRA_DIST += mbchar.h ## end gnulib module mbchar ## begin gnulib module mbrtowc EXTRA_DIST += mbrtowc.c EXTRA_libgnu_la_SOURCES += mbrtowc.c ## end gnulib module mbrtowc ## begin gnulib module mbschr libgnu_la_SOURCES += mbschr.c ## end gnulib module mbschr ## begin gnulib module mbsinit EXTRA_DIST += mbsinit.c EXTRA_libgnu_la_SOURCES += mbsinit.c ## end gnulib module mbsinit ## begin gnulib module mbspbrk libgnu_la_SOURCES += mbspbrk.c ## end gnulib module mbspbrk ## begin gnulib module mbsspn libgnu_la_SOURCES += mbsspn.c ## end gnulib module mbsspn ## begin gnulib module mbstok_r libgnu_la_SOURCES += mbstok_r.c ## end gnulib module mbstok_r ## begin gnulib module mbtowc EXTRA_DIST += mbtowc-impl.h mbtowc.c EXTRA_libgnu_la_SOURCES += mbtowc.c ## end gnulib module mbtowc ## begin gnulib module mbuiter libgnu_la_SOURCES += mbuiter.h mbuiter.c ## end gnulib module mbuiter ## begin gnulib module memchr EXTRA_DIST += memchr.c memchr.valgrind EXTRA_libgnu_la_SOURCES += memchr.c ## end gnulib module memchr ## begin gnulib module mempcpy EXTRA_DIST += mempcpy.c EXTRA_libgnu_la_SOURCES += mempcpy.c ## end gnulib module mempcpy ## begin gnulib module minmax libgnu_la_SOURCES += minmax.h ## end gnulib module minmax ## begin gnulib module msvc-inval EXTRA_DIST += msvc-inval.c msvc-inval.h EXTRA_libgnu_la_SOURCES += msvc-inval.c ## end gnulib module msvc-inval ## begin gnulib module msvc-nothrow EXTRA_DIST += msvc-nothrow.c msvc-nothrow.h EXTRA_libgnu_la_SOURCES += msvc-nothrow.c ## end gnulib module msvc-nothrow ## begin gnulib module nl_langinfo EXTRA_DIST += nl_langinfo.c EXTRA_libgnu_la_SOURCES += nl_langinfo.c ## end gnulib module nl_langinfo ## begin gnulib module nproc libgnu_la_SOURCES += nproc.c EXTRA_DIST += nproc.h ## end gnulib module nproc ## begin gnulib module rawmemchr EXTRA_DIST += rawmemchr.c rawmemchr.valgrind EXTRA_libgnu_la_SOURCES += rawmemchr.c ## end gnulib module rawmemchr ## begin gnulib module regex EXTRA_DIST += regcomp.c regex.c regex.h regex_internal.c regex_internal.h regexec.c EXTRA_libgnu_la_SOURCES += regcomp.c regex.c regex_internal.c regexec.c ## end gnulib module regex ## begin gnulib module size_max libgnu_la_SOURCES += size_max.h ## end gnulib module size_max ## begin gnulib module sleep EXTRA_DIST += sleep.c EXTRA_libgnu_la_SOURCES += sleep.c ## end gnulib module sleep ## begin gnulib module snippet/_Noreturn # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. _NORETURN_H=$(srcdir)/_Noreturn.h EXTRA_DIST += _Noreturn.h ## end gnulib module snippet/_Noreturn ## begin gnulib module snippet/arg-nonnull # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. ARG_NONNULL_H=$(srcdir)/arg-nonnull.h EXTRA_DIST += arg-nonnull.h ## end gnulib module snippet/arg-nonnull ## begin gnulib module snippet/c++defs # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. CXXDEFS_H=$(srcdir)/c++defs.h EXTRA_DIST += c++defs.h ## end gnulib module snippet/c++defs ## begin gnulib module snippet/warn-on-use # Because this Makefile snippet defines a variable used by other # gnulib Makefile snippets, it must be present in all makefiles that # need it. This is ensured by the applicability 'all' defined above. WARN_ON_USE_H=$(srcdir)/warn-on-use.h EXTRA_DIST += warn-on-use.h ## end gnulib module snippet/warn-on-use ## begin gnulib module stdalign BUILT_SOURCES += $(STDALIGN_H) # We need the following in order to create when the system # doesn't have one that works. if GL_GENERATE_STDALIGN_H stdalign.h: stdalign.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/stdalign.in.h; \ } > $@-t && \ mv $@-t $@ else stdalign.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stdalign.h stdalign.h-t EXTRA_DIST += stdalign.in.h ## end gnulib module stdalign ## begin gnulib module stdbool BUILT_SOURCES += $(STDBOOL_H) # We need the following in order to create when the system # doesn't have one that works. if GL_GENERATE_STDBOOL_H stdbool.h: stdbool.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's/@''HAVE__BOOL''@/$(HAVE__BOOL)/g' < $(srcdir)/stdbool.in.h; \ } > $@-t && \ mv $@-t $@ else stdbool.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stdbool.h stdbool.h-t EXTRA_DIST += stdbool.in.h ## end gnulib module stdbool ## begin gnulib module stddef BUILT_SOURCES += $(STDDEF_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_STDDEF_H stddef.h: stddef.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDDEF_H''@|$(NEXT_STDDEF_H)|g' \ -e 's|@''HAVE_MAX_ALIGN_T''@|$(HAVE_MAX_ALIGN_T)|g' \ -e 's|@''HAVE_WCHAR_T''@|$(HAVE_WCHAR_T)|g' \ -e 's|@''REPLACE_NULL''@|$(REPLACE_NULL)|g' \ < $(srcdir)/stddef.in.h; \ } > $@-t && \ mv $@-t $@ else stddef.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stddef.h stddef.h-t EXTRA_DIST += stddef.in.h ## end gnulib module stddef ## begin gnulib module stdint BUILT_SOURCES += $(STDINT_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_STDINT_H stdint.h: stdint.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_STDINT_H''@/$(HAVE_STDINT_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDINT_H''@|$(NEXT_STDINT_H)|g' \ -e 's/@''HAVE_C99_STDINT_H''@/$(HAVE_C99_STDINT_H)/g' \ -e 's/@''HAVE_SYS_TYPES_H''@/$(HAVE_SYS_TYPES_H)/g' \ -e 's/@''HAVE_INTTYPES_H''@/$(HAVE_INTTYPES_H)/g' \ -e 's/@''HAVE_SYS_INTTYPES_H''@/$(HAVE_SYS_INTTYPES_H)/g' \ -e 's/@''HAVE_SYS_BITYPES_H''@/$(HAVE_SYS_BITYPES_H)/g' \ -e 's/@''HAVE_WCHAR_H''@/$(HAVE_WCHAR_H)/g' \ -e 's/@''HAVE_LONG_LONG_INT''@/$(HAVE_LONG_LONG_INT)/g' \ -e 's/@''HAVE_UNSIGNED_LONG_LONG_INT''@/$(HAVE_UNSIGNED_LONG_LONG_INT)/g' \ -e 's/@''APPLE_UNIVERSAL_BUILD''@/$(APPLE_UNIVERSAL_BUILD)/g' \ -e 's/@''BITSIZEOF_PTRDIFF_T''@/$(BITSIZEOF_PTRDIFF_T)/g' \ -e 's/@''PTRDIFF_T_SUFFIX''@/$(PTRDIFF_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_SIG_ATOMIC_T''@/$(BITSIZEOF_SIG_ATOMIC_T)/g' \ -e 's/@''HAVE_SIGNED_SIG_ATOMIC_T''@/$(HAVE_SIGNED_SIG_ATOMIC_T)/g' \ -e 's/@''SIG_ATOMIC_T_SUFFIX''@/$(SIG_ATOMIC_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_SIZE_T''@/$(BITSIZEOF_SIZE_T)/g' \ -e 's/@''SIZE_T_SUFFIX''@/$(SIZE_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_WCHAR_T''@/$(BITSIZEOF_WCHAR_T)/g' \ -e 's/@''HAVE_SIGNED_WCHAR_T''@/$(HAVE_SIGNED_WCHAR_T)/g' \ -e 's/@''WCHAR_T_SUFFIX''@/$(WCHAR_T_SUFFIX)/g' \ -e 's/@''BITSIZEOF_WINT_T''@/$(BITSIZEOF_WINT_T)/g' \ -e 's/@''HAVE_SIGNED_WINT_T''@/$(HAVE_SIGNED_WINT_T)/g' \ -e 's/@''WINT_T_SUFFIX''@/$(WINT_T_SUFFIX)/g' \ -e 's/@''GNULIB_OVERRIDES_WINT_T''@/$(GNULIB_OVERRIDES_WINT_T)/g' \ < $(srcdir)/stdint.in.h; \ } > $@-t && \ mv $@-t $@ else stdint.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += stdint.h stdint.h-t EXTRA_DIST += stdint.in.h ## end gnulib module stdint ## begin gnulib module stdio BUILT_SOURCES += stdio.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdio.h: stdio.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDIO_H''@|$(NEXT_STDIO_H)|g' \ -e 's/@''GNULIB_DPRINTF''@/$(GNULIB_DPRINTF)/g' \ -e 's/@''GNULIB_FCLOSE''@/$(GNULIB_FCLOSE)/g' \ -e 's/@''GNULIB_FDOPEN''@/$(GNULIB_FDOPEN)/g' \ -e 's/@''GNULIB_FFLUSH''@/$(GNULIB_FFLUSH)/g' \ -e 's/@''GNULIB_FGETC''@/$(GNULIB_FGETC)/g' \ -e 's/@''GNULIB_FGETS''@/$(GNULIB_FGETS)/g' \ -e 's/@''GNULIB_FOPEN''@/$(GNULIB_FOPEN)/g' \ -e 's/@''GNULIB_FPRINTF''@/$(GNULIB_FPRINTF)/g' \ -e 's/@''GNULIB_FPRINTF_POSIX''@/$(GNULIB_FPRINTF_POSIX)/g' \ -e 's/@''GNULIB_FPURGE''@/$(GNULIB_FPURGE)/g' \ -e 's/@''GNULIB_FPUTC''@/$(GNULIB_FPUTC)/g' \ -e 's/@''GNULIB_FPUTS''@/$(GNULIB_FPUTS)/g' \ -e 's/@''GNULIB_FREAD''@/$(GNULIB_FREAD)/g' \ -e 's/@''GNULIB_FREOPEN''@/$(GNULIB_FREOPEN)/g' \ -e 's/@''GNULIB_FSCANF''@/$(GNULIB_FSCANF)/g' \ -e 's/@''GNULIB_FSEEK''@/$(GNULIB_FSEEK)/g' \ -e 's/@''GNULIB_FSEEKO''@/$(GNULIB_FSEEKO)/g' \ -e 's/@''GNULIB_FTELL''@/$(GNULIB_FTELL)/g' \ -e 's/@''GNULIB_FTELLO''@/$(GNULIB_FTELLO)/g' \ -e 's/@''GNULIB_FWRITE''@/$(GNULIB_FWRITE)/g' \ -e 's/@''GNULIB_GETC''@/$(GNULIB_GETC)/g' \ -e 's/@''GNULIB_GETCHAR''@/$(GNULIB_GETCHAR)/g' \ -e 's/@''GNULIB_GETDELIM''@/$(GNULIB_GETDELIM)/g' \ -e 's/@''GNULIB_GETLINE''@/$(GNULIB_GETLINE)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF''@/$(GNULIB_OBSTACK_PRINTF)/g' \ -e 's/@''GNULIB_OBSTACK_PRINTF_POSIX''@/$(GNULIB_OBSTACK_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PCLOSE''@/$(GNULIB_PCLOSE)/g' \ -e 's/@''GNULIB_PERROR''@/$(GNULIB_PERROR)/g' \ -e 's/@''GNULIB_POPEN''@/$(GNULIB_POPEN)/g' \ -e 's/@''GNULIB_PRINTF''@/$(GNULIB_PRINTF)/g' \ -e 's/@''GNULIB_PRINTF_POSIX''@/$(GNULIB_PRINTF_POSIX)/g' \ -e 's/@''GNULIB_PUTC''@/$(GNULIB_PUTC)/g' \ -e 's/@''GNULIB_PUTCHAR''@/$(GNULIB_PUTCHAR)/g' \ -e 's/@''GNULIB_PUTS''@/$(GNULIB_PUTS)/g' \ -e 's/@''GNULIB_REMOVE''@/$(GNULIB_REMOVE)/g' \ -e 's/@''GNULIB_RENAME''@/$(GNULIB_RENAME)/g' \ -e 's/@''GNULIB_RENAMEAT''@/$(GNULIB_RENAMEAT)/g' \ -e 's/@''GNULIB_SCANF''@/$(GNULIB_SCANF)/g' \ -e 's/@''GNULIB_SNPRINTF''@/$(GNULIB_SNPRINTF)/g' \ -e 's/@''GNULIB_SPRINTF_POSIX''@/$(GNULIB_SPRINTF_POSIX)/g' \ -e 's/@''GNULIB_STDIO_H_NONBLOCKING''@/$(GNULIB_STDIO_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_STDIO_H_SIGPIPE''@/$(GNULIB_STDIO_H_SIGPIPE)/g' \ -e 's/@''GNULIB_TMPFILE''@/$(GNULIB_TMPFILE)/g' \ -e 's/@''GNULIB_VASPRINTF''@/$(GNULIB_VASPRINTF)/g' \ -e 's/@''GNULIB_VDPRINTF''@/$(GNULIB_VDPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF''@/$(GNULIB_VFPRINTF)/g' \ -e 's/@''GNULIB_VFPRINTF_POSIX''@/$(GNULIB_VFPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VFSCANF''@/$(GNULIB_VFSCANF)/g' \ -e 's/@''GNULIB_VSCANF''@/$(GNULIB_VSCANF)/g' \ -e 's/@''GNULIB_VPRINTF''@/$(GNULIB_VPRINTF)/g' \ -e 's/@''GNULIB_VPRINTF_POSIX''@/$(GNULIB_VPRINTF_POSIX)/g' \ -e 's/@''GNULIB_VSNPRINTF''@/$(GNULIB_VSNPRINTF)/g' \ -e 's/@''GNULIB_VSPRINTF_POSIX''@/$(GNULIB_VSPRINTF_POSIX)/g' \ < $(srcdir)/stdio.in.h | \ sed -e 's|@''HAVE_DECL_FPURGE''@|$(HAVE_DECL_FPURGE)|g' \ -e 's|@''HAVE_DECL_FSEEKO''@|$(HAVE_DECL_FSEEKO)|g' \ -e 's|@''HAVE_DECL_FTELLO''@|$(HAVE_DECL_FTELLO)|g' \ -e 's|@''HAVE_DECL_GETDELIM''@|$(HAVE_DECL_GETDELIM)|g' \ -e 's|@''HAVE_DECL_GETLINE''@|$(HAVE_DECL_GETLINE)|g' \ -e 's|@''HAVE_DECL_OBSTACK_PRINTF''@|$(HAVE_DECL_OBSTACK_PRINTF)|g' \ -e 's|@''HAVE_DECL_SNPRINTF''@|$(HAVE_DECL_SNPRINTF)|g' \ -e 's|@''HAVE_DECL_VSNPRINTF''@|$(HAVE_DECL_VSNPRINTF)|g' \ -e 's|@''HAVE_DPRINTF''@|$(HAVE_DPRINTF)|g' \ -e 's|@''HAVE_FSEEKO''@|$(HAVE_FSEEKO)|g' \ -e 's|@''HAVE_FTELLO''@|$(HAVE_FTELLO)|g' \ -e 's|@''HAVE_PCLOSE''@|$(HAVE_PCLOSE)|g' \ -e 's|@''HAVE_POPEN''@|$(HAVE_POPEN)|g' \ -e 's|@''HAVE_RENAMEAT''@|$(HAVE_RENAMEAT)|g' \ -e 's|@''HAVE_VASPRINTF''@|$(HAVE_VASPRINTF)|g' \ -e 's|@''HAVE_VDPRINTF''@|$(HAVE_VDPRINTF)|g' \ -e 's|@''REPLACE_DPRINTF''@|$(REPLACE_DPRINTF)|g' \ -e 's|@''REPLACE_FCLOSE''@|$(REPLACE_FCLOSE)|g' \ -e 's|@''REPLACE_FDOPEN''@|$(REPLACE_FDOPEN)|g' \ -e 's|@''REPLACE_FFLUSH''@|$(REPLACE_FFLUSH)|g' \ -e 's|@''REPLACE_FOPEN''@|$(REPLACE_FOPEN)|g' \ -e 's|@''REPLACE_FPRINTF''@|$(REPLACE_FPRINTF)|g' \ -e 's|@''REPLACE_FPURGE''@|$(REPLACE_FPURGE)|g' \ -e 's|@''REPLACE_FREOPEN''@|$(REPLACE_FREOPEN)|g' \ -e 's|@''REPLACE_FSEEK''@|$(REPLACE_FSEEK)|g' \ -e 's|@''REPLACE_FSEEKO''@|$(REPLACE_FSEEKO)|g' \ -e 's|@''REPLACE_FTELL''@|$(REPLACE_FTELL)|g' \ -e 's|@''REPLACE_FTELLO''@|$(REPLACE_FTELLO)|g' \ -e 's|@''REPLACE_GETDELIM''@|$(REPLACE_GETDELIM)|g' \ -e 's|@''REPLACE_GETLINE''@|$(REPLACE_GETLINE)|g' \ -e 's|@''REPLACE_OBSTACK_PRINTF''@|$(REPLACE_OBSTACK_PRINTF)|g' \ -e 's|@''REPLACE_PERROR''@|$(REPLACE_PERROR)|g' \ -e 's|@''REPLACE_POPEN''@|$(REPLACE_POPEN)|g' \ -e 's|@''REPLACE_PRINTF''@|$(REPLACE_PRINTF)|g' \ -e 's|@''REPLACE_REMOVE''@|$(REPLACE_REMOVE)|g' \ -e 's|@''REPLACE_RENAME''@|$(REPLACE_RENAME)|g' \ -e 's|@''REPLACE_RENAMEAT''@|$(REPLACE_RENAMEAT)|g' \ -e 's|@''REPLACE_SNPRINTF''@|$(REPLACE_SNPRINTF)|g' \ -e 's|@''REPLACE_SPRINTF''@|$(REPLACE_SPRINTF)|g' \ -e 's|@''REPLACE_STDIO_READ_FUNCS''@|$(REPLACE_STDIO_READ_FUNCS)|g' \ -e 's|@''REPLACE_STDIO_WRITE_FUNCS''@|$(REPLACE_STDIO_WRITE_FUNCS)|g' \ -e 's|@''REPLACE_TMPFILE''@|$(REPLACE_TMPFILE)|g' \ -e 's|@''REPLACE_VASPRINTF''@|$(REPLACE_VASPRINTF)|g' \ -e 's|@''REPLACE_VDPRINTF''@|$(REPLACE_VDPRINTF)|g' \ -e 's|@''REPLACE_VFPRINTF''@|$(REPLACE_VFPRINTF)|g' \ -e 's|@''REPLACE_VPRINTF''@|$(REPLACE_VPRINTF)|g' \ -e 's|@''REPLACE_VSNPRINTF''@|$(REPLACE_VSNPRINTF)|g' \ -e 's|@''REPLACE_VSPRINTF''@|$(REPLACE_VSPRINTF)|g' \ -e 's|@''ASM_SYMBOL_PREFIX''@|$(ASM_SYMBOL_PREFIX)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += stdio.h stdio.h-t EXTRA_DIST += stdio.in.h ## end gnulib module stdio ## begin gnulib module stdlib BUILT_SOURCES += stdlib.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. stdlib.h: stdlib.in.h $(top_builddir)/config.status $(CXXDEFS_H) \ $(_NORETURN_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STDLIB_H''@|$(NEXT_STDLIB_H)|g' \ -e 's/@''GNULIB__EXIT''@/$(GNULIB__EXIT)/g' \ -e 's/@''GNULIB_ATOLL''@/$(GNULIB_ATOLL)/g' \ -e 's/@''GNULIB_CALLOC_POSIX''@/$(GNULIB_CALLOC_POSIX)/g' \ -e 's/@''GNULIB_CANONICALIZE_FILE_NAME''@/$(GNULIB_CANONICALIZE_FILE_NAME)/g' \ -e 's/@''GNULIB_GETLOADAVG''@/$(GNULIB_GETLOADAVG)/g' \ -e 's/@''GNULIB_GETSUBOPT''@/$(GNULIB_GETSUBOPT)/g' \ -e 's/@''GNULIB_GRANTPT''@/$(GNULIB_GRANTPT)/g' \ -e 's/@''GNULIB_MALLOC_POSIX''@/$(GNULIB_MALLOC_POSIX)/g' \ -e 's/@''GNULIB_MBTOWC''@/$(GNULIB_MBTOWC)/g' \ -e 's/@''GNULIB_MKDTEMP''@/$(GNULIB_MKDTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMP''@/$(GNULIB_MKOSTEMP)/g' \ -e 's/@''GNULIB_MKOSTEMPS''@/$(GNULIB_MKOSTEMPS)/g' \ -e 's/@''GNULIB_MKSTEMP''@/$(GNULIB_MKSTEMP)/g' \ -e 's/@''GNULIB_MKSTEMPS''@/$(GNULIB_MKSTEMPS)/g' \ -e 's/@''GNULIB_POSIX_OPENPT''@/$(GNULIB_POSIX_OPENPT)/g' \ -e 's/@''GNULIB_PTSNAME''@/$(GNULIB_PTSNAME)/g' \ -e 's/@''GNULIB_PTSNAME_R''@/$(GNULIB_PTSNAME_R)/g' \ -e 's/@''GNULIB_PUTENV''@/$(GNULIB_PUTENV)/g' \ -e 's/@''GNULIB_QSORT_R''@/$(GNULIB_QSORT_R)/g' \ -e 's/@''GNULIB_RANDOM''@/$(GNULIB_RANDOM)/g' \ -e 's/@''GNULIB_RANDOM_R''@/$(GNULIB_RANDOM_R)/g' \ -e 's/@''GNULIB_REALLOC_POSIX''@/$(GNULIB_REALLOC_POSIX)/g' \ -e 's/@''GNULIB_REALLOCARRAY''@/$(GNULIB_REALLOCARRAY)/g' \ -e 's/@''GNULIB_REALPATH''@/$(GNULIB_REALPATH)/g' \ -e 's/@''GNULIB_RPMATCH''@/$(GNULIB_RPMATCH)/g' \ -e 's/@''GNULIB_SECURE_GETENV''@/$(GNULIB_SECURE_GETENV)/g' \ -e 's/@''GNULIB_SETENV''@/$(GNULIB_SETENV)/g' \ -e 's/@''GNULIB_STRTOD''@/$(GNULIB_STRTOD)/g' \ -e 's/@''GNULIB_STRTOLL''@/$(GNULIB_STRTOLL)/g' \ -e 's/@''GNULIB_STRTOULL''@/$(GNULIB_STRTOULL)/g' \ -e 's/@''GNULIB_SYSTEM_POSIX''@/$(GNULIB_SYSTEM_POSIX)/g' \ -e 's/@''GNULIB_UNLOCKPT''@/$(GNULIB_UNLOCKPT)/g' \ -e 's/@''GNULIB_UNSETENV''@/$(GNULIB_UNSETENV)/g' \ -e 's/@''GNULIB_WCTOMB''@/$(GNULIB_WCTOMB)/g' \ < $(srcdir)/stdlib.in.h | \ sed -e 's|@''HAVE__EXIT''@|$(HAVE__EXIT)|g' \ -e 's|@''HAVE_ATOLL''@|$(HAVE_ATOLL)|g' \ -e 's|@''HAVE_CANONICALIZE_FILE_NAME''@|$(HAVE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''HAVE_DECL_GETLOADAVG''@|$(HAVE_DECL_GETLOADAVG)|g' \ -e 's|@''HAVE_GETSUBOPT''@|$(HAVE_GETSUBOPT)|g' \ -e 's|@''HAVE_GRANTPT''@|$(HAVE_GRANTPT)|g' \ -e 's|@''HAVE_DECL_INITSTATE''@|$(HAVE_DECL_INITSTATE)|g' \ -e 's|@''HAVE_MKDTEMP''@|$(HAVE_MKDTEMP)|g' \ -e 's|@''HAVE_MKOSTEMP''@|$(HAVE_MKOSTEMP)|g' \ -e 's|@''HAVE_MKOSTEMPS''@|$(HAVE_MKOSTEMPS)|g' \ -e 's|@''HAVE_MKSTEMP''@|$(HAVE_MKSTEMP)|g' \ -e 's|@''HAVE_MKSTEMPS''@|$(HAVE_MKSTEMPS)|g' \ -e 's|@''HAVE_POSIX_OPENPT''@|$(HAVE_POSIX_OPENPT)|g' \ -e 's|@''HAVE_PTSNAME''@|$(HAVE_PTSNAME)|g' \ -e 's|@''HAVE_PTSNAME_R''@|$(HAVE_PTSNAME_R)|g' \ -e 's|@''HAVE_QSORT_R''@|$(HAVE_QSORT_R)|g' \ -e 's|@''HAVE_RANDOM''@|$(HAVE_RANDOM)|g' \ -e 's|@''HAVE_RANDOM_H''@|$(HAVE_RANDOM_H)|g' \ -e 's|@''HAVE_RANDOM_R''@|$(HAVE_RANDOM_R)|g' \ -e 's|@''HAVE_REALLOCARRAY''@|$(HAVE_REALLOCARRAY)|g' \ -e 's|@''HAVE_REALPATH''@|$(HAVE_REALPATH)|g' \ -e 's|@''HAVE_RPMATCH''@|$(HAVE_RPMATCH)|g' \ -e 's|@''HAVE_SECURE_GETENV''@|$(HAVE_SECURE_GETENV)|g' \ -e 's|@''HAVE_DECL_SETENV''@|$(HAVE_DECL_SETENV)|g' \ -e 's|@''HAVE_DECL_SETSTATE''@|$(HAVE_DECL_SETSTATE)|g' \ -e 's|@''HAVE_STRTOD''@|$(HAVE_STRTOD)|g' \ -e 's|@''HAVE_STRTOLL''@|$(HAVE_STRTOLL)|g' \ -e 's|@''HAVE_STRTOULL''@|$(HAVE_STRTOULL)|g' \ -e 's|@''HAVE_STRUCT_RANDOM_DATA''@|$(HAVE_STRUCT_RANDOM_DATA)|g' \ -e 's|@''HAVE_SYS_LOADAVG_H''@|$(HAVE_SYS_LOADAVG_H)|g' \ -e 's|@''HAVE_UNLOCKPT''@|$(HAVE_UNLOCKPT)|g' \ -e 's|@''HAVE_DECL_UNSETENV''@|$(HAVE_DECL_UNSETENV)|g' \ -e 's|@''REPLACE_CALLOC''@|$(REPLACE_CALLOC)|g' \ -e 's|@''REPLACE_CANONICALIZE_FILE_NAME''@|$(REPLACE_CANONICALIZE_FILE_NAME)|g' \ -e 's|@''REPLACE_MALLOC''@|$(REPLACE_MALLOC)|g' \ -e 's|@''REPLACE_MBTOWC''@|$(REPLACE_MBTOWC)|g' \ -e 's|@''REPLACE_MKSTEMP''@|$(REPLACE_MKSTEMP)|g' \ -e 's|@''REPLACE_PTSNAME''@|$(REPLACE_PTSNAME)|g' \ -e 's|@''REPLACE_PTSNAME_R''@|$(REPLACE_PTSNAME_R)|g' \ -e 's|@''REPLACE_PUTENV''@|$(REPLACE_PUTENV)|g' \ -e 's|@''REPLACE_QSORT_R''@|$(REPLACE_QSORT_R)|g' \ -e 's|@''REPLACE_RANDOM_R''@|$(REPLACE_RANDOM_R)|g' \ -e 's|@''REPLACE_REALLOC''@|$(REPLACE_REALLOC)|g' \ -e 's|@''REPLACE_REALPATH''@|$(REPLACE_REALPATH)|g' \ -e 's|@''REPLACE_SETENV''@|$(REPLACE_SETENV)|g' \ -e 's|@''REPLACE_STRTOD''@|$(REPLACE_STRTOD)|g' \ -e 's|@''REPLACE_UNSETENV''@|$(REPLACE_UNSETENV)|g' \ -e 's|@''REPLACE_WCTOMB''@|$(REPLACE_WCTOMB)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _Noreturn/r $(_NORETURN_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += stdlib.h stdlib.h-t EXTRA_DIST += stdlib.in.h ## end gnulib module stdlib ## begin gnulib module strcase EXTRA_DIST += strcasecmp.c strncasecmp.c EXTRA_libgnu_la_SOURCES += strcasecmp.c strncasecmp.c ## end gnulib module strcase ## begin gnulib module strchrnul EXTRA_DIST += strchrnul.c strchrnul.valgrind EXTRA_libgnu_la_SOURCES += strchrnul.c ## end gnulib module strchrnul ## begin gnulib module streq EXTRA_DIST += streq.h ## end gnulib module streq ## begin gnulib module strerror EXTRA_DIST += strerror.c EXTRA_libgnu_la_SOURCES += strerror.c ## end gnulib module strerror ## begin gnulib module strerror-override EXTRA_DIST += strerror-override.c strerror-override.h EXTRA_libgnu_la_SOURCES += strerror-override.c ## end gnulib module strerror-override ## begin gnulib module string BUILT_SOURCES += string.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. string.h: string.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRING_H''@|$(NEXT_STRING_H)|g' \ -e 's/@''GNULIB_EXPLICIT_BZERO''@/$(GNULIB_EXPLICIT_BZERO)/g' \ -e 's/@''GNULIB_FFSL''@/$(GNULIB_FFSL)/g' \ -e 's/@''GNULIB_FFSLL''@/$(GNULIB_FFSLL)/g' \ -e 's/@''GNULIB_MBSLEN''@/$(GNULIB_MBSLEN)/g' \ -e 's/@''GNULIB_MBSNLEN''@/$(GNULIB_MBSNLEN)/g' \ -e 's/@''GNULIB_MBSCHR''@/$(GNULIB_MBSCHR)/g' \ -e 's/@''GNULIB_MBSRCHR''@/$(GNULIB_MBSRCHR)/g' \ -e 's/@''GNULIB_MBSSTR''@/$(GNULIB_MBSSTR)/g' \ -e 's/@''GNULIB_MBSCASECMP''@/$(GNULIB_MBSCASECMP)/g' \ -e 's/@''GNULIB_MBSNCASECMP''@/$(GNULIB_MBSNCASECMP)/g' \ -e 's/@''GNULIB_MBSPCASECMP''@/$(GNULIB_MBSPCASECMP)/g' \ -e 's/@''GNULIB_MBSCASESTR''@/$(GNULIB_MBSCASESTR)/g' \ -e 's/@''GNULIB_MBSCSPN''@/$(GNULIB_MBSCSPN)/g' \ -e 's/@''GNULIB_MBSPBRK''@/$(GNULIB_MBSPBRK)/g' \ -e 's/@''GNULIB_MBSSPN''@/$(GNULIB_MBSSPN)/g' \ -e 's/@''GNULIB_MBSSEP''@/$(GNULIB_MBSSEP)/g' \ -e 's/@''GNULIB_MBSTOK_R''@/$(GNULIB_MBSTOK_R)/g' \ -e 's/@''GNULIB_MEMCHR''@/$(GNULIB_MEMCHR)/g' \ -e 's/@''GNULIB_MEMMEM''@/$(GNULIB_MEMMEM)/g' \ -e 's/@''GNULIB_MEMPCPY''@/$(GNULIB_MEMPCPY)/g' \ -e 's/@''GNULIB_MEMRCHR''@/$(GNULIB_MEMRCHR)/g' \ -e 's/@''GNULIB_RAWMEMCHR''@/$(GNULIB_RAWMEMCHR)/g' \ -e 's/@''GNULIB_STPCPY''@/$(GNULIB_STPCPY)/g' \ -e 's/@''GNULIB_STPNCPY''@/$(GNULIB_STPNCPY)/g' \ -e 's/@''GNULIB_STRCHRNUL''@/$(GNULIB_STRCHRNUL)/g' \ -e 's/@''GNULIB_STRDUP''@/$(GNULIB_STRDUP)/g' \ -e 's/@''GNULIB_STRNCAT''@/$(GNULIB_STRNCAT)/g' \ -e 's/@''GNULIB_STRNDUP''@/$(GNULIB_STRNDUP)/g' \ -e 's/@''GNULIB_STRNLEN''@/$(GNULIB_STRNLEN)/g' \ -e 's/@''GNULIB_STRPBRK''@/$(GNULIB_STRPBRK)/g' \ -e 's/@''GNULIB_STRSEP''@/$(GNULIB_STRSEP)/g' \ -e 's/@''GNULIB_STRSTR''@/$(GNULIB_STRSTR)/g' \ -e 's/@''GNULIB_STRCASESTR''@/$(GNULIB_STRCASESTR)/g' \ -e 's/@''GNULIB_STRTOK_R''@/$(GNULIB_STRTOK_R)/g' \ -e 's/@''GNULIB_STRERROR''@/$(GNULIB_STRERROR)/g' \ -e 's/@''GNULIB_STRERROR_R''@/$(GNULIB_STRERROR_R)/g' \ -e 's/@''GNULIB_STRSIGNAL''@/$(GNULIB_STRSIGNAL)/g' \ -e 's/@''GNULIB_STRVERSCMP''@/$(GNULIB_STRVERSCMP)/g' \ < $(srcdir)/string.in.h | \ sed -e 's|@''HAVE_EXPLICIT_BZERO''@|$(HAVE_EXPLICIT_BZERO)|g' \ -e 's|@''HAVE_FFSL''@|$(HAVE_FFSL)|g' \ -e 's|@''HAVE_FFSLL''@|$(HAVE_FFSLL)|g' \ -e 's|@''HAVE_MBSLEN''@|$(HAVE_MBSLEN)|g' \ -e 's|@''HAVE_MEMCHR''@|$(HAVE_MEMCHR)|g' \ -e 's|@''HAVE_DECL_MEMMEM''@|$(HAVE_DECL_MEMMEM)|g' \ -e 's|@''HAVE_MEMPCPY''@|$(HAVE_MEMPCPY)|g' \ -e 's|@''HAVE_DECL_MEMRCHR''@|$(HAVE_DECL_MEMRCHR)|g' \ -e 's|@''HAVE_RAWMEMCHR''@|$(HAVE_RAWMEMCHR)|g' \ -e 's|@''HAVE_STPCPY''@|$(HAVE_STPCPY)|g' \ -e 's|@''HAVE_STPNCPY''@|$(HAVE_STPNCPY)|g' \ -e 's|@''HAVE_STRCHRNUL''@|$(HAVE_STRCHRNUL)|g' \ -e 's|@''HAVE_DECL_STRDUP''@|$(HAVE_DECL_STRDUP)|g' \ -e 's|@''HAVE_DECL_STRNDUP''@|$(HAVE_DECL_STRNDUP)|g' \ -e 's|@''HAVE_DECL_STRNLEN''@|$(HAVE_DECL_STRNLEN)|g' \ -e 's|@''HAVE_STRPBRK''@|$(HAVE_STRPBRK)|g' \ -e 's|@''HAVE_STRSEP''@|$(HAVE_STRSEP)|g' \ -e 's|@''HAVE_STRCASESTR''@|$(HAVE_STRCASESTR)|g' \ -e 's|@''HAVE_DECL_STRTOK_R''@|$(HAVE_DECL_STRTOK_R)|g' \ -e 's|@''HAVE_DECL_STRERROR_R''@|$(HAVE_DECL_STRERROR_R)|g' \ -e 's|@''HAVE_DECL_STRSIGNAL''@|$(HAVE_DECL_STRSIGNAL)|g' \ -e 's|@''HAVE_STRVERSCMP''@|$(HAVE_STRVERSCMP)|g' \ -e 's|@''REPLACE_MEMCHR''@|$(REPLACE_MEMCHR)|g' \ -e 's|@''REPLACE_MEMMEM''@|$(REPLACE_MEMMEM)|g' \ -e 's|@''REPLACE_STPNCPY''@|$(REPLACE_STPNCPY)|g' \ -e 's|@''REPLACE_STRCHRNUL''@|$(REPLACE_STRCHRNUL)|g' \ -e 's|@''REPLACE_STRDUP''@|$(REPLACE_STRDUP)|g' \ -e 's|@''REPLACE_STRNCAT''@|$(REPLACE_STRNCAT)|g' \ -e 's|@''REPLACE_STRNDUP''@|$(REPLACE_STRNDUP)|g' \ -e 's|@''REPLACE_STRNLEN''@|$(REPLACE_STRNLEN)|g' \ -e 's|@''REPLACE_STRSTR''@|$(REPLACE_STRSTR)|g' \ -e 's|@''REPLACE_STRCASESTR''@|$(REPLACE_STRCASESTR)|g' \ -e 's|@''REPLACE_STRTOK_R''@|$(REPLACE_STRTOK_R)|g' \ -e 's|@''REPLACE_STRERROR''@|$(REPLACE_STRERROR)|g' \ -e 's|@''REPLACE_STRERROR_R''@|$(REPLACE_STRERROR_R)|g' \ -e 's|@''REPLACE_STRSIGNAL''@|$(REPLACE_STRSIGNAL)|g' \ -e 's|@''UNDEFINE_STRTOK_R''@|$(UNDEFINE_STRTOK_R)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ < $(srcdir)/string.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += string.h string.h-t EXTRA_DIST += string.in.h ## end gnulib module string ## begin gnulib module strings BUILT_SOURCES += strings.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. strings.h: strings.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(ARG_NONNULL_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */' && \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_STRINGS_H''@|$(HAVE_STRINGS_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_STRINGS_H''@|$(NEXT_STRINGS_H)|g' \ -e 's|@''GNULIB_FFS''@|$(GNULIB_FFS)|g' \ -e 's|@''HAVE_FFS''@|$(HAVE_FFS)|g' \ -e 's|@''HAVE_STRCASECMP''@|$(HAVE_STRCASECMP)|g' \ -e 's|@''HAVE_DECL_STRNCASECMP''@|$(HAVE_DECL_STRNCASECMP)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/strings.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += strings.h strings.h-t EXTRA_DIST += strings.in.h ## end gnulib module strings ## begin gnulib module strndup EXTRA_DIST += strndup.c EXTRA_libgnu_la_SOURCES += strndup.c ## end gnulib module strndup ## begin gnulib module strnlen EXTRA_DIST += strnlen.c EXTRA_libgnu_la_SOURCES += strnlen.c ## end gnulib module strnlen ## begin gnulib module strnlen1 libgnu_la_SOURCES += strnlen1.h strnlen1.c ## end gnulib module strnlen1 ## begin gnulib module strtod EXTRA_DIST += strtod.c EXTRA_libgnu_la_SOURCES += strtod.c ## end gnulib module strtod ## begin gnulib module strtok_r EXTRA_DIST += strtok_r.c EXTRA_libgnu_la_SOURCES += strtok_r.c ## end gnulib module strtok_r ## begin gnulib module sys_types BUILT_SOURCES += sys/types.h # We need the following in order to create when the system # doesn't have one that works with the given compiler. sys/types.h: sys_types.in.h $(top_builddir)/config.status $(AM_V_at)$(MKDIR_P) sys $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYS_TYPES_H''@|$(NEXT_SYS_TYPES_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ -e 's|@''WINDOWS_STAT_INODES''@|$(WINDOWS_STAT_INODES)|g' \ < $(srcdir)/sys_types.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += sys/types.h sys/types.h-t EXTRA_DIST += sys_types.in.h ## end gnulib module sys_types ## begin gnulib module sysexits BUILT_SOURCES += $(SYSEXITS_H) # We need the following in order to create when the system # doesn't have one that works with the given compiler. if GL_GENERATE_SYSEXITS_H sysexits.h: sysexits.in.h $(top_builddir)/config.status $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_SYSEXITS_H''@|$(HAVE_SYSEXITS_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_SYSEXITS_H''@|$(NEXT_SYSEXITS_H)|g' \ < $(srcdir)/sysexits.in.h; \ } > $@-t && \ mv -f $@-t $@ else sysexits.h: $(top_builddir)/config.status rm -f $@ endif MOSTLYCLEANFILES += sysexits.h sysexits.h-t EXTRA_DIST += sysexits.in.h ## end gnulib module sysexits ## begin gnulib module threadlib libgnu_la_SOURCES += glthread/threadlib.c EXTRA_DIST += $(top_srcdir)/bootstrapped/build-aux/config.rpath ## end gnulib module threadlib ## begin gnulib module unistd BUILT_SOURCES += unistd.h libgnu_la_SOURCES += unistd.c # We need the following in order to create an empty placeholder for # when the system doesn't have one. unistd.h: unistd.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''HAVE_UNISTD_H''@|$(HAVE_UNISTD_H)|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_UNISTD_H''@|$(NEXT_UNISTD_H)|g' \ -e 's|@''WINDOWS_64_BIT_OFF_T''@|$(WINDOWS_64_BIT_OFF_T)|g' \ -e 's/@''GNULIB_CHDIR''@/$(GNULIB_CHDIR)/g' \ -e 's/@''GNULIB_CHOWN''@/$(GNULIB_CHOWN)/g' \ -e 's/@''GNULIB_CLOSE''@/$(GNULIB_CLOSE)/g' \ -e 's/@''GNULIB_DUP''@/$(GNULIB_DUP)/g' \ -e 's/@''GNULIB_DUP2''@/$(GNULIB_DUP2)/g' \ -e 's/@''GNULIB_DUP3''@/$(GNULIB_DUP3)/g' \ -e 's/@''GNULIB_ENVIRON''@/$(GNULIB_ENVIRON)/g' \ -e 's/@''GNULIB_EUIDACCESS''@/$(GNULIB_EUIDACCESS)/g' \ -e 's/@''GNULIB_FACCESSAT''@/$(GNULIB_FACCESSAT)/g' \ -e 's/@''GNULIB_FCHDIR''@/$(GNULIB_FCHDIR)/g' \ -e 's/@''GNULIB_FCHOWNAT''@/$(GNULIB_FCHOWNAT)/g' \ -e 's/@''GNULIB_FDATASYNC''@/$(GNULIB_FDATASYNC)/g' \ -e 's/@''GNULIB_FSYNC''@/$(GNULIB_FSYNC)/g' \ -e 's/@''GNULIB_FTRUNCATE''@/$(GNULIB_FTRUNCATE)/g' \ -e 's/@''GNULIB_GETCWD''@/$(GNULIB_GETCWD)/g' \ -e 's/@''GNULIB_GETDOMAINNAME''@/$(GNULIB_GETDOMAINNAME)/g' \ -e 's/@''GNULIB_GETDTABLESIZE''@/$(GNULIB_GETDTABLESIZE)/g' \ -e 's/@''GNULIB_GETGROUPS''@/$(GNULIB_GETGROUPS)/g' \ -e 's/@''GNULIB_GETHOSTNAME''@/$(GNULIB_GETHOSTNAME)/g' \ -e 's/@''GNULIB_GETLOGIN''@/$(GNULIB_GETLOGIN)/g' \ -e 's/@''GNULIB_GETLOGIN_R''@/$(GNULIB_GETLOGIN_R)/g' \ -e 's/@''GNULIB_GETPAGESIZE''@/$(GNULIB_GETPAGESIZE)/g' \ -e 's/@''GNULIB_GETUSERSHELL''@/$(GNULIB_GETUSERSHELL)/g' \ -e 's/@''GNULIB_GROUP_MEMBER''@/$(GNULIB_GROUP_MEMBER)/g' \ -e 's/@''GNULIB_ISATTY''@/$(GNULIB_ISATTY)/g' \ -e 's/@''GNULIB_LCHOWN''@/$(GNULIB_LCHOWN)/g' \ -e 's/@''GNULIB_LINK''@/$(GNULIB_LINK)/g' \ -e 's/@''GNULIB_LINKAT''@/$(GNULIB_LINKAT)/g' \ -e 's/@''GNULIB_LSEEK''@/$(GNULIB_LSEEK)/g' \ -e 's/@''GNULIB_PIPE''@/$(GNULIB_PIPE)/g' \ -e 's/@''GNULIB_PIPE2''@/$(GNULIB_PIPE2)/g' \ -e 's/@''GNULIB_PREAD''@/$(GNULIB_PREAD)/g' \ -e 's/@''GNULIB_PWRITE''@/$(GNULIB_PWRITE)/g' \ -e 's/@''GNULIB_READ''@/$(GNULIB_READ)/g' \ -e 's/@''GNULIB_READLINK''@/$(GNULIB_READLINK)/g' \ -e 's/@''GNULIB_READLINKAT''@/$(GNULIB_READLINKAT)/g' \ -e 's/@''GNULIB_RMDIR''@/$(GNULIB_RMDIR)/g' \ -e 's/@''GNULIB_SETHOSTNAME''@/$(GNULIB_SETHOSTNAME)/g' \ -e 's/@''GNULIB_SLEEP''@/$(GNULIB_SLEEP)/g' \ -e 's/@''GNULIB_SYMLINK''@/$(GNULIB_SYMLINK)/g' \ -e 's/@''GNULIB_SYMLINKAT''@/$(GNULIB_SYMLINKAT)/g' \ -e 's/@''GNULIB_TRUNCATE''@/$(GNULIB_TRUNCATE)/g' \ -e 's/@''GNULIB_TTYNAME_R''@/$(GNULIB_TTYNAME_R)/g' \ -e 's/@''GNULIB_UNISTD_H_GETOPT''@/0$(GNULIB_GL_UNISTD_H_GETOPT)/g' \ -e 's/@''GNULIB_UNISTD_H_NONBLOCKING''@/$(GNULIB_UNISTD_H_NONBLOCKING)/g' \ -e 's/@''GNULIB_UNISTD_H_SIGPIPE''@/$(GNULIB_UNISTD_H_SIGPIPE)/g' \ -e 's/@''GNULIB_UNLINK''@/$(GNULIB_UNLINK)/g' \ -e 's/@''GNULIB_UNLINKAT''@/$(GNULIB_UNLINKAT)/g' \ -e 's/@''GNULIB_USLEEP''@/$(GNULIB_USLEEP)/g' \ -e 's/@''GNULIB_WRITE''@/$(GNULIB_WRITE)/g' \ < $(srcdir)/unistd.in.h | \ sed -e 's|@''HAVE_CHOWN''@|$(HAVE_CHOWN)|g' \ -e 's|@''HAVE_DUP2''@|$(HAVE_DUP2)|g' \ -e 's|@''HAVE_DUP3''@|$(HAVE_DUP3)|g' \ -e 's|@''HAVE_EUIDACCESS''@|$(HAVE_EUIDACCESS)|g' \ -e 's|@''HAVE_FACCESSAT''@|$(HAVE_FACCESSAT)|g' \ -e 's|@''HAVE_FCHDIR''@|$(HAVE_FCHDIR)|g' \ -e 's|@''HAVE_FCHOWNAT''@|$(HAVE_FCHOWNAT)|g' \ -e 's|@''HAVE_FDATASYNC''@|$(HAVE_FDATASYNC)|g' \ -e 's|@''HAVE_FSYNC''@|$(HAVE_FSYNC)|g' \ -e 's|@''HAVE_FTRUNCATE''@|$(HAVE_FTRUNCATE)|g' \ -e 's|@''HAVE_GETDTABLESIZE''@|$(HAVE_GETDTABLESIZE)|g' \ -e 's|@''HAVE_GETGROUPS''@|$(HAVE_GETGROUPS)|g' \ -e 's|@''HAVE_GETHOSTNAME''@|$(HAVE_GETHOSTNAME)|g' \ -e 's|@''HAVE_GETPAGESIZE''@|$(HAVE_GETPAGESIZE)|g' \ -e 's|@''HAVE_GROUP_MEMBER''@|$(HAVE_GROUP_MEMBER)|g' \ -e 's|@''HAVE_LCHOWN''@|$(HAVE_LCHOWN)|g' \ -e 's|@''HAVE_LINK''@|$(HAVE_LINK)|g' \ -e 's|@''HAVE_LINKAT''@|$(HAVE_LINKAT)|g' \ -e 's|@''HAVE_PIPE''@|$(HAVE_PIPE)|g' \ -e 's|@''HAVE_PIPE2''@|$(HAVE_PIPE2)|g' \ -e 's|@''HAVE_PREAD''@|$(HAVE_PREAD)|g' \ -e 's|@''HAVE_PWRITE''@|$(HAVE_PWRITE)|g' \ -e 's|@''HAVE_READLINK''@|$(HAVE_READLINK)|g' \ -e 's|@''HAVE_READLINKAT''@|$(HAVE_READLINKAT)|g' \ -e 's|@''HAVE_SETHOSTNAME''@|$(HAVE_SETHOSTNAME)|g' \ -e 's|@''HAVE_SLEEP''@|$(HAVE_SLEEP)|g' \ -e 's|@''HAVE_SYMLINK''@|$(HAVE_SYMLINK)|g' \ -e 's|@''HAVE_SYMLINKAT''@|$(HAVE_SYMLINKAT)|g' \ -e 's|@''HAVE_TRUNCATE''@|$(HAVE_TRUNCATE)|g' \ -e 's|@''HAVE_UNLINKAT''@|$(HAVE_UNLINKAT)|g' \ -e 's|@''HAVE_USLEEP''@|$(HAVE_USLEEP)|g' \ -e 's|@''HAVE_DECL_ENVIRON''@|$(HAVE_DECL_ENVIRON)|g' \ -e 's|@''HAVE_DECL_FCHDIR''@|$(HAVE_DECL_FCHDIR)|g' \ -e 's|@''HAVE_DECL_FDATASYNC''@|$(HAVE_DECL_FDATASYNC)|g' \ -e 's|@''HAVE_DECL_GETDOMAINNAME''@|$(HAVE_DECL_GETDOMAINNAME)|g' \ -e 's|@''HAVE_DECL_GETLOGIN''@|$(HAVE_DECL_GETLOGIN)|g' \ -e 's|@''HAVE_DECL_GETLOGIN_R''@|$(HAVE_DECL_GETLOGIN_R)|g' \ -e 's|@''HAVE_DECL_GETPAGESIZE''@|$(HAVE_DECL_GETPAGESIZE)|g' \ -e 's|@''HAVE_DECL_GETUSERSHELL''@|$(HAVE_DECL_GETUSERSHELL)|g' \ -e 's|@''HAVE_DECL_SETHOSTNAME''@|$(HAVE_DECL_SETHOSTNAME)|g' \ -e 's|@''HAVE_DECL_TTYNAME_R''@|$(HAVE_DECL_TTYNAME_R)|g' \ -e 's|@''HAVE_OS_H''@|$(HAVE_OS_H)|g' \ -e 's|@''HAVE_SYS_PARAM_H''@|$(HAVE_SYS_PARAM_H)|g' \ | \ sed -e 's|@''REPLACE_CHOWN''@|$(REPLACE_CHOWN)|g' \ -e 's|@''REPLACE_CLOSE''@|$(REPLACE_CLOSE)|g' \ -e 's|@''REPLACE_DUP''@|$(REPLACE_DUP)|g' \ -e 's|@''REPLACE_DUP2''@|$(REPLACE_DUP2)|g' \ -e 's|@''REPLACE_FACCESSAT''@|$(REPLACE_FACCESSAT)|g' \ -e 's|@''REPLACE_FCHOWNAT''@|$(REPLACE_FCHOWNAT)|g' \ -e 's|@''REPLACE_FTRUNCATE''@|$(REPLACE_FTRUNCATE)|g' \ -e 's|@''REPLACE_GETCWD''@|$(REPLACE_GETCWD)|g' \ -e 's|@''REPLACE_GETDOMAINNAME''@|$(REPLACE_GETDOMAINNAME)|g' \ -e 's|@''REPLACE_GETDTABLESIZE''@|$(REPLACE_GETDTABLESIZE)|g' \ -e 's|@''REPLACE_GETLOGIN_R''@|$(REPLACE_GETLOGIN_R)|g' \ -e 's|@''REPLACE_GETGROUPS''@|$(REPLACE_GETGROUPS)|g' \ -e 's|@''REPLACE_GETPAGESIZE''@|$(REPLACE_GETPAGESIZE)|g' \ -e 's|@''REPLACE_ISATTY''@|$(REPLACE_ISATTY)|g' \ -e 's|@''REPLACE_LCHOWN''@|$(REPLACE_LCHOWN)|g' \ -e 's|@''REPLACE_LINK''@|$(REPLACE_LINK)|g' \ -e 's|@''REPLACE_LINKAT''@|$(REPLACE_LINKAT)|g' \ -e 's|@''REPLACE_LSEEK''@|$(REPLACE_LSEEK)|g' \ -e 's|@''REPLACE_PREAD''@|$(REPLACE_PREAD)|g' \ -e 's|@''REPLACE_PWRITE''@|$(REPLACE_PWRITE)|g' \ -e 's|@''REPLACE_READ''@|$(REPLACE_READ)|g' \ -e 's|@''REPLACE_READLINK''@|$(REPLACE_READLINK)|g' \ -e 's|@''REPLACE_READLINKAT''@|$(REPLACE_READLINKAT)|g' \ -e 's|@''REPLACE_RMDIR''@|$(REPLACE_RMDIR)|g' \ -e 's|@''REPLACE_SLEEP''@|$(REPLACE_SLEEP)|g' \ -e 's|@''REPLACE_SYMLINK''@|$(REPLACE_SYMLINK)|g' \ -e 's|@''REPLACE_SYMLINKAT''@|$(REPLACE_SYMLINKAT)|g' \ -e 's|@''REPLACE_TRUNCATE''@|$(REPLACE_TRUNCATE)|g' \ -e 's|@''REPLACE_TTYNAME_R''@|$(REPLACE_TTYNAME_R)|g' \ -e 's|@''REPLACE_UNLINK''@|$(REPLACE_UNLINK)|g' \ -e 's|@''REPLACE_UNLINKAT''@|$(REPLACE_UNLINKAT)|g' \ -e 's|@''REPLACE_USLEEP''@|$(REPLACE_USLEEP)|g' \ -e 's|@''REPLACE_WRITE''@|$(REPLACE_WRITE)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H''@|$(UNISTD_H_HAVE_WINSOCK2_H)|g' \ -e 's|@''UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS''@|$(UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += unistd.h unistd.h-t EXTRA_DIST += unistd.in.h ## end gnulib module unistd ## begin gnulib module unitypes BUILT_SOURCES += $(LIBUNISTRING_UNITYPES_H) unitypes.h: unitypes.in.h $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/unitypes.in.h; \ } > $@-t && \ mv -f $@-t $@ MOSTLYCLEANFILES += unitypes.h unitypes.h-t EXTRA_DIST += unitypes.in.h ## end gnulib module unitypes ## begin gnulib module uniwidth/base BUILT_SOURCES += $(LIBUNISTRING_UNIWIDTH_H) uniwidth.h: uniwidth.in.h $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ cat $(srcdir)/uniwidth.in.h; \ } > $@-t && \ mv -f $@-t $@ MOSTLYCLEANFILES += uniwidth.h uniwidth.h-t EXTRA_DIST += localcharset.h uniwidth.in.h ## end gnulib module uniwidth/base ## begin gnulib module uniwidth/width if LIBUNISTRING_COMPILE_UNIWIDTH_WIDTH libgnu_la_SOURCES += uniwidth/width.c endif EXTRA_DIST += uniwidth/cjk.h ## end gnulib module uniwidth/width ## begin gnulib module vasnprintf EXTRA_DIST += asnprintf.c float+.h printf-args.c printf-args.h printf-parse.c printf-parse.h vasnprintf.c vasnprintf.h EXTRA_libgnu_la_SOURCES += asnprintf.c printf-args.c printf-parse.c vasnprintf.c ## end gnulib module vasnprintf ## begin gnulib module verify EXTRA_DIST += verify.h ## end gnulib module verify ## begin gnulib module vsnprintf EXTRA_DIST += vsnprintf.c EXTRA_libgnu_la_SOURCES += vsnprintf.c ## end gnulib module vsnprintf ## begin gnulib module wchar BUILT_SOURCES += wchar.h # We need the following in order to create when the system # version does not work standalone. wchar.h: wchar.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(ARG_NONNULL_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''HAVE_FEATURES_H''@|$(HAVE_FEATURES_H)|g' \ -e 's|@''NEXT_WCHAR_H''@|$(NEXT_WCHAR_H)|g' \ -e 's|@''HAVE_WCHAR_H''@|$(HAVE_WCHAR_H)|g' \ -e 's/@''HAVE_CRTDEFS_H''@/$(HAVE_CRTDEFS_H)/g' \ -e 's/@''GNULIB_OVERRIDES_WINT_T''@/$(GNULIB_OVERRIDES_WINT_T)/g' \ -e 's/@''GNULIB_BTOWC''@/$(GNULIB_BTOWC)/g' \ -e 's/@''GNULIB_WCTOB''@/$(GNULIB_WCTOB)/g' \ -e 's/@''GNULIB_MBSINIT''@/$(GNULIB_MBSINIT)/g' \ -e 's/@''GNULIB_MBRTOWC''@/$(GNULIB_MBRTOWC)/g' \ -e 's/@''GNULIB_MBRLEN''@/$(GNULIB_MBRLEN)/g' \ -e 's/@''GNULIB_MBSRTOWCS''@/$(GNULIB_MBSRTOWCS)/g' \ -e 's/@''GNULIB_MBSNRTOWCS''@/$(GNULIB_MBSNRTOWCS)/g' \ -e 's/@''GNULIB_WCRTOMB''@/$(GNULIB_WCRTOMB)/g' \ -e 's/@''GNULIB_WCSRTOMBS''@/$(GNULIB_WCSRTOMBS)/g' \ -e 's/@''GNULIB_WCSNRTOMBS''@/$(GNULIB_WCSNRTOMBS)/g' \ -e 's/@''GNULIB_WCWIDTH''@/$(GNULIB_WCWIDTH)/g' \ -e 's/@''GNULIB_WMEMCHR''@/$(GNULIB_WMEMCHR)/g' \ -e 's/@''GNULIB_WMEMCMP''@/$(GNULIB_WMEMCMP)/g' \ -e 's/@''GNULIB_WMEMCPY''@/$(GNULIB_WMEMCPY)/g' \ -e 's/@''GNULIB_WMEMMOVE''@/$(GNULIB_WMEMMOVE)/g' \ -e 's/@''GNULIB_WMEMSET''@/$(GNULIB_WMEMSET)/g' \ -e 's/@''GNULIB_WCSLEN''@/$(GNULIB_WCSLEN)/g' \ -e 's/@''GNULIB_WCSNLEN''@/$(GNULIB_WCSNLEN)/g' \ -e 's/@''GNULIB_WCSCPY''@/$(GNULIB_WCSCPY)/g' \ -e 's/@''GNULIB_WCPCPY''@/$(GNULIB_WCPCPY)/g' \ -e 's/@''GNULIB_WCSNCPY''@/$(GNULIB_WCSNCPY)/g' \ -e 's/@''GNULIB_WCPNCPY''@/$(GNULIB_WCPNCPY)/g' \ -e 's/@''GNULIB_WCSCAT''@/$(GNULIB_WCSCAT)/g' \ -e 's/@''GNULIB_WCSNCAT''@/$(GNULIB_WCSNCAT)/g' \ -e 's/@''GNULIB_WCSCMP''@/$(GNULIB_WCSCMP)/g' \ -e 's/@''GNULIB_WCSNCMP''@/$(GNULIB_WCSNCMP)/g' \ -e 's/@''GNULIB_WCSCASECMP''@/$(GNULIB_WCSCASECMP)/g' \ -e 's/@''GNULIB_WCSNCASECMP''@/$(GNULIB_WCSNCASECMP)/g' \ -e 's/@''GNULIB_WCSCOLL''@/$(GNULIB_WCSCOLL)/g' \ -e 's/@''GNULIB_WCSXFRM''@/$(GNULIB_WCSXFRM)/g' \ -e 's/@''GNULIB_WCSDUP''@/$(GNULIB_WCSDUP)/g' \ -e 's/@''GNULIB_WCSCHR''@/$(GNULIB_WCSCHR)/g' \ -e 's/@''GNULIB_WCSRCHR''@/$(GNULIB_WCSRCHR)/g' \ -e 's/@''GNULIB_WCSCSPN''@/$(GNULIB_WCSCSPN)/g' \ -e 's/@''GNULIB_WCSSPN''@/$(GNULIB_WCSSPN)/g' \ -e 's/@''GNULIB_WCSPBRK''@/$(GNULIB_WCSPBRK)/g' \ -e 's/@''GNULIB_WCSSTR''@/$(GNULIB_WCSSTR)/g' \ -e 's/@''GNULIB_WCSTOK''@/$(GNULIB_WCSTOK)/g' \ -e 's/@''GNULIB_WCSWIDTH''@/$(GNULIB_WCSWIDTH)/g' \ -e 's/@''GNULIB_WCSFTIME''@/$(GNULIB_WCSFTIME)/g' \ < $(srcdir)/wchar.in.h | \ sed -e 's|@''HAVE_WINT_T''@|$(HAVE_WINT_T)|g' \ -e 's|@''HAVE_BTOWC''@|$(HAVE_BTOWC)|g' \ -e 's|@''HAVE_MBSINIT''@|$(HAVE_MBSINIT)|g' \ -e 's|@''HAVE_MBRTOWC''@|$(HAVE_MBRTOWC)|g' \ -e 's|@''HAVE_MBRLEN''@|$(HAVE_MBRLEN)|g' \ -e 's|@''HAVE_MBSRTOWCS''@|$(HAVE_MBSRTOWCS)|g' \ -e 's|@''HAVE_MBSNRTOWCS''@|$(HAVE_MBSNRTOWCS)|g' \ -e 's|@''HAVE_WCRTOMB''@|$(HAVE_WCRTOMB)|g' \ -e 's|@''HAVE_WCSRTOMBS''@|$(HAVE_WCSRTOMBS)|g' \ -e 's|@''HAVE_WCSNRTOMBS''@|$(HAVE_WCSNRTOMBS)|g' \ -e 's|@''HAVE_WMEMCHR''@|$(HAVE_WMEMCHR)|g' \ -e 's|@''HAVE_WMEMCMP''@|$(HAVE_WMEMCMP)|g' \ -e 's|@''HAVE_WMEMCPY''@|$(HAVE_WMEMCPY)|g' \ -e 's|@''HAVE_WMEMMOVE''@|$(HAVE_WMEMMOVE)|g' \ -e 's|@''HAVE_WMEMSET''@|$(HAVE_WMEMSET)|g' \ -e 's|@''HAVE_WCSLEN''@|$(HAVE_WCSLEN)|g' \ -e 's|@''HAVE_WCSNLEN''@|$(HAVE_WCSNLEN)|g' \ -e 's|@''HAVE_WCSCPY''@|$(HAVE_WCSCPY)|g' \ -e 's|@''HAVE_WCPCPY''@|$(HAVE_WCPCPY)|g' \ -e 's|@''HAVE_WCSNCPY''@|$(HAVE_WCSNCPY)|g' \ -e 's|@''HAVE_WCPNCPY''@|$(HAVE_WCPNCPY)|g' \ -e 's|@''HAVE_WCSCAT''@|$(HAVE_WCSCAT)|g' \ -e 's|@''HAVE_WCSNCAT''@|$(HAVE_WCSNCAT)|g' \ -e 's|@''HAVE_WCSCMP''@|$(HAVE_WCSCMP)|g' \ -e 's|@''HAVE_WCSNCMP''@|$(HAVE_WCSNCMP)|g' \ -e 's|@''HAVE_WCSCASECMP''@|$(HAVE_WCSCASECMP)|g' \ -e 's|@''HAVE_WCSNCASECMP''@|$(HAVE_WCSNCASECMP)|g' \ -e 's|@''HAVE_WCSCOLL''@|$(HAVE_WCSCOLL)|g' \ -e 's|@''HAVE_WCSXFRM''@|$(HAVE_WCSXFRM)|g' \ -e 's|@''HAVE_WCSDUP''@|$(HAVE_WCSDUP)|g' \ -e 's|@''HAVE_WCSCHR''@|$(HAVE_WCSCHR)|g' \ -e 's|@''HAVE_WCSRCHR''@|$(HAVE_WCSRCHR)|g' \ -e 's|@''HAVE_WCSCSPN''@|$(HAVE_WCSCSPN)|g' \ -e 's|@''HAVE_WCSSPN''@|$(HAVE_WCSSPN)|g' \ -e 's|@''HAVE_WCSPBRK''@|$(HAVE_WCSPBRK)|g' \ -e 's|@''HAVE_WCSSTR''@|$(HAVE_WCSSTR)|g' \ -e 's|@''HAVE_WCSTOK''@|$(HAVE_WCSTOK)|g' \ -e 's|@''HAVE_WCSWIDTH''@|$(HAVE_WCSWIDTH)|g' \ -e 's|@''HAVE_WCSFTIME''@|$(HAVE_WCSFTIME)|g' \ -e 's|@''HAVE_DECL_WCTOB''@|$(HAVE_DECL_WCTOB)|g' \ -e 's|@''HAVE_DECL_WCWIDTH''@|$(HAVE_DECL_WCWIDTH)|g' \ | \ sed -e 's|@''REPLACE_MBSTATE_T''@|$(REPLACE_MBSTATE_T)|g' \ -e 's|@''REPLACE_BTOWC''@|$(REPLACE_BTOWC)|g' \ -e 's|@''REPLACE_WCTOB''@|$(REPLACE_WCTOB)|g' \ -e 's|@''REPLACE_MBSINIT''@|$(REPLACE_MBSINIT)|g' \ -e 's|@''REPLACE_MBRTOWC''@|$(REPLACE_MBRTOWC)|g' \ -e 's|@''REPLACE_MBRLEN''@|$(REPLACE_MBRLEN)|g' \ -e 's|@''REPLACE_MBSRTOWCS''@|$(REPLACE_MBSRTOWCS)|g' \ -e 's|@''REPLACE_MBSNRTOWCS''@|$(REPLACE_MBSNRTOWCS)|g' \ -e 's|@''REPLACE_WCRTOMB''@|$(REPLACE_WCRTOMB)|g' \ -e 's|@''REPLACE_WCSRTOMBS''@|$(REPLACE_WCSRTOMBS)|g' \ -e 's|@''REPLACE_WCSNRTOMBS''@|$(REPLACE_WCSNRTOMBS)|g' \ -e 's|@''REPLACE_WCWIDTH''@|$(REPLACE_WCWIDTH)|g' \ -e 's|@''REPLACE_WCSWIDTH''@|$(REPLACE_WCSWIDTH)|g' \ -e 's|@''REPLACE_WCSFTIME''@|$(REPLACE_WCSFTIME)|g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_ARG_NONNULL/r $(ARG_NONNULL_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)'; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += wchar.h wchar.h-t EXTRA_DIST += wchar.in.h ## end gnulib module wchar ## begin gnulib module wcrtomb EXTRA_DIST += wcrtomb.c EXTRA_libgnu_la_SOURCES += wcrtomb.c ## end gnulib module wcrtomb ## begin gnulib module wctype-h BUILT_SOURCES += wctype.h libgnu_la_SOURCES += wctype-h.c # We need the following in order to create when the system # doesn't have one that works with the given compiler. wctype.h: wctype.in.h $(top_builddir)/config.status $(CXXDEFS_H) $(WARN_ON_USE_H) $(AM_V_GEN)rm -f $@-t $@ && \ { echo '/* DO NOT EDIT! GENERATED AUTOMATICALLY! */'; \ sed -e 's|@''GUARD_PREFIX''@|GL|g' \ -e 's/@''HAVE_WCTYPE_H''@/$(HAVE_WCTYPE_H)/g' \ -e 's|@''INCLUDE_NEXT''@|$(INCLUDE_NEXT)|g' \ -e 's|@''PRAGMA_SYSTEM_HEADER''@|@PRAGMA_SYSTEM_HEADER@|g' \ -e 's|@''PRAGMA_COLUMNS''@|@PRAGMA_COLUMNS@|g' \ -e 's|@''NEXT_WCTYPE_H''@|$(NEXT_WCTYPE_H)|g' \ -e 's/@''HAVE_CRTDEFS_H''@/$(HAVE_CRTDEFS_H)/g' \ -e 's/@''GNULIB_OVERRIDES_WINT_T''@/$(GNULIB_OVERRIDES_WINT_T)/g' \ -e 's/@''GNULIB_ISWBLANK''@/$(GNULIB_ISWBLANK)/g' \ -e 's/@''GNULIB_WCTYPE''@/$(GNULIB_WCTYPE)/g' \ -e 's/@''GNULIB_ISWCTYPE''@/$(GNULIB_ISWCTYPE)/g' \ -e 's/@''GNULIB_WCTRANS''@/$(GNULIB_WCTRANS)/g' \ -e 's/@''GNULIB_TOWCTRANS''@/$(GNULIB_TOWCTRANS)/g' \ -e 's/@''HAVE_ISWBLANK''@/$(HAVE_ISWBLANK)/g' \ -e 's/@''HAVE_ISWCNTRL''@/$(HAVE_ISWCNTRL)/g' \ -e 's/@''HAVE_WCTYPE_T''@/$(HAVE_WCTYPE_T)/g' \ -e 's/@''HAVE_WCTRANS_T''@/$(HAVE_WCTRANS_T)/g' \ -e 's/@''HAVE_WINT_T''@/$(HAVE_WINT_T)/g' \ -e 's/@''REPLACE_ISWBLANK''@/$(REPLACE_ISWBLANK)/g' \ -e 's/@''REPLACE_ISWCNTRL''@/$(REPLACE_ISWCNTRL)/g' \ -e 's/@''REPLACE_TOWLOWER''@/$(REPLACE_TOWLOWER)/g' \ -e '/definitions of _GL_FUNCDECL_RPL/r $(CXXDEFS_H)' \ -e '/definition of _GL_WARN_ON_USE/r $(WARN_ON_USE_H)' \ < $(srcdir)/wctype.in.h; \ } > $@-t && \ mv $@-t $@ MOSTLYCLEANFILES += wctype.h wctype.h-t EXTRA_DIST += wctype.in.h ## end gnulib module wctype-h ## begin gnulib module wcwidth EXTRA_DIST += wcwidth.c EXTRA_libgnu_la_SOURCES += wcwidth.c ## end gnulib module wcwidth ## begin gnulib module xsize libgnu_la_SOURCES += xsize.h xsize.c ## end gnulib module xsize mostlyclean-local: mostlyclean-generic @for dir in '' $(MOSTLYCLEANDIRS); do \ if test -n "$$dir" && test -d $$dir; then \ echo "rmdir $$dir"; rmdir $$dir; \ fi; \ done; \ : gnuastro-0.5/bootstrapped/lib/uniwidth/0000755000175000017500000000000013217220465015332 500000000000000gnuastro-0.5/bootstrapped/lib/uniwidth/cjk.h0000644000175000017500000000314613217200021016160 00000000000000/* Test for CJK encoding. Copyright (C) 2001-2002, 2005-2007, 2009-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2002. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include "streq.h" static int is_cjk_encoding (const char *encoding) { if (0 /* Legacy Japanese encodings */ || STREQ_OPT (encoding, "EUC-JP", 'E', 'U', 'C', '-', 'J', 'P', 0, 0, 0) /* Legacy Chinese encodings */ || STREQ_OPT (encoding, "GB2312", 'G', 'B', '2', '3', '1', '2', 0, 0, 0) || STREQ_OPT (encoding, "GBK", 'G', 'B', 'K', 0, 0, 0, 0, 0, 0) || STREQ_OPT (encoding, "EUC-TW", 'E', 'U', 'C', '-', 'T', 'W', 0, 0, 0) || STREQ_OPT (encoding, "BIG5", 'B', 'I', 'G', '5', 0, 0, 0, 0, 0) /* Legacy Korean encodings */ || STREQ_OPT (encoding, "EUC-KR", 'E', 'U', 'C', '-', 'K', 'R', 0, 0, 0) || STREQ_OPT (encoding, "CP949", 'C', 'P', '9', '4', '9', 0, 0, 0, 0) || STREQ_OPT (encoding, "JOHAB", 'J', 'O', 'H', 'A', 'B', 0, 0, 0, 0)) return 1; return 0; } gnuastro-0.5/bootstrapped/lib/uniwidth/width.c0000644000175000017500000006554113217200021016532 00000000000000/* Determine display width of Unicode character. Copyright (C) 2001-2002, 2006-2017 Free Software Foundation, Inc. Written by Bruno Haible , 2002. This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . */ #include /* Specification. */ #include "uniwidth.h" #include "cjk.h" /* * Non-spacing attribute table. * Consists of: * - Non-spacing characters; generated from PropList.txt or * "grep '^[^;]*;[^;]*;[^;]*;[^;]*;NSM;' UnicodeData.txt" * - Format control characters; generated from * "grep '^[^;]*;[^;]*;Cf;' UnicodeData.txt" * - Zero width characters; generated from * "grep '^[^;]*;ZERO WIDTH ' UnicodeData.txt" */ static const unsigned char nonspacing_table_data[38*64] = { /* 0x0000-0x01ff */ 0xff, 0xff, 0xff, 0xff, 0x00, 0x00, 0x00, 0x00, /* 0x0000-0x003f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, /* 0x0040-0x007f */ 0xff, 0xff, 0xff, 0xff, 0x00, 0x20, 0x00, 0x00, /* 0x0080-0x00bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x00c0-0x00ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0100-0x013f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0140-0x017f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0180-0x01bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x01c0-0x01ff */ /* 0x0200-0x03ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0200-0x023f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0240-0x027f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0280-0x02bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x02c0-0x02ff */ 0xff, 0xff, 0xff, 0xff, 0xff, 0xff, 0xff, 0xff, /* 0x0300-0x033f */ 0xff, 0xff, 0xff, 0xff, 0xff, 0xff, 0x00, 0x00, /* 0x0340-0x037f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0380-0x03bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x03c0-0x03ff */ /* 0x0400-0x05ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0400-0x043f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0440-0x047f */ 0xf8, 0x03, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0480-0x04bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x04c0-0x04ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0500-0x053f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0540-0x057f */ 0x00, 0x00, 0xfe, 0xff, 0xff, 0xff, 0xff, 0xbf, /* 0x0580-0x05bf */ 0xb6, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x05c0-0x05ff */ /* 0x0600-0x07ff */ 0x3f, 0x00, 0xff, 0x17, 0x00, 0x00, 0x00, 0x00, /* 0x0600-0x063f */ 0x00, 0xf8, 0xff, 0xff, 0x00, 0x00, 0x01, 0x00, /* 0x0640-0x067f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0680-0x06bf */ 0x00, 0x00, 0xc0, 0xbf, 0x9f, 0x3d, 0x00, 0x00, /* 0x06c0-0x06ff */ 0x00, 0x80, 0x02, 0x00, 0x00, 0x00, 0xff, 0xff, /* 0x0700-0x073f */ 0xff, 0x07, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0740-0x077f */ 0x00, 0x00, 0x00, 0x00, 0xc0, 0xff, 0x01, 0x00, /* 0x0780-0x07bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0xf8, 0x0f, 0x00, /* 0x07c0-0x07ff */ /* 0x0800-0x09ff */ 0x00, 0x00, 0xc0, 0xfb, 0xef, 0x3e, 0x00, 0x00, /* 0x0800-0x083f */ 0x00, 0x00, 0x00, 0x0e, 0x00, 0x00, 0x00, 0x00, /* 0x0840-0x087f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0880-0x08bf */ 0x00, 0x00, 0xf0, 0xff, 0xff, 0xff, 0xff, 0xff, /* 0x08c0-0x08ff */ 0x07, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x14, /* 0x0900-0x093f */ 0xfe, 0x21, 0xfe, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x0940-0x097f */ 0x02, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x10, /* 0x0980-0x09bf */ 0x1e, 0x20, 0x00, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x09c0-0x09ff */ /* 0x0a00-0x0bff */ 0x06, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x10, /* 0x0a00-0x0a3f */ 0x86, 0x39, 0x02, 0x00, 0x00, 0x00, 0x23, 0x00, /* 0x0a40-0x0a7f */ 0x06, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x10, /* 0x0a80-0x0abf */ 0xbe, 0x21, 0x00, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x0ac0-0x0aff */ 0x02, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x90, /* 0x0b00-0x0b3f */ 0x1e, 0x20, 0x40, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x0b40-0x0b7f */ 0x04, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0b80-0x0bbf */ 0x01, 0x20, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0bc0-0x0bff */ /* 0x0c00-0x0dff */ 0x01, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xc0, /* 0x0c00-0x0c3f */ 0xc1, 0x3d, 0x60, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x0c40-0x0c7f */ 0x02, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x10, /* 0x0c80-0x0cbf */ 0x00, 0x30, 0x00, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x0cc0-0x0cff */ 0x02, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0d00-0x0d3f */ 0x1e, 0x20, 0x00, 0x00, 0x0c, 0x00, 0x00, 0x00, /* 0x0d40-0x0d7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0d80-0x0dbf */ 0x00, 0x04, 0x5c, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0dc0-0x0dff */ /* 0x0e00-0x0fff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xf2, 0x07, /* 0x0e00-0x0e3f */ 0x80, 0x7f, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0e40-0x0e7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xf2, 0x1b, /* 0x0e80-0x0ebf */ 0x00, 0x3f, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0ec0-0x0eff */ 0x00, 0x00, 0x00, 0x03, 0x00, 0x00, 0xa0, 0x02, /* 0x0f00-0x0f3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xfe, 0x7f, /* 0x0f40-0x0f7f */ 0xdf, 0xe0, 0xff, 0xfe, 0xff, 0xff, 0xff, 0x1f, /* 0x0f80-0x0fbf */ 0x40, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x0fc0-0x0fff */ /* 0x1000-0x11ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0xe0, 0xfd, 0x66, /* 0x1000-0x103f */ 0x00, 0x00, 0x00, 0xc3, 0x01, 0x00, 0x1e, 0x00, /* 0x1040-0x107f */ 0x64, 0x20, 0x00, 0x20, 0x00, 0x00, 0x00, 0x00, /* 0x1080-0x10bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10c0-0x10ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1100-0x113f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1140-0x117f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1180-0x11bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11c0-0x11ff */ /* 0x1200-0x13ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1200-0x123f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1240-0x127f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1280-0x12bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x12c0-0x12ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1300-0x133f */ 0x00, 0x00, 0x00, 0xe0, 0x00, 0x00, 0x00, 0x00, /* 0x1340-0x137f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1380-0x13bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x13c0-0x13ff */ /* 0x1600-0x17ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1600-0x163f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1640-0x167f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1680-0x16bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16c0-0x16ff */ 0x00, 0x00, 0x1c, 0x00, 0x00, 0x00, 0x1c, 0x00, /* 0x1700-0x173f */ 0x00, 0x00, 0x0c, 0x00, 0x00, 0x00, 0x0c, 0x00, /* 0x1740-0x177f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xb0, 0x3f, /* 0x1780-0x17bf */ 0x40, 0xfe, 0x0f, 0x20, 0x00, 0x00, 0x00, 0x00, /* 0x17c0-0x17ff */ /* 0x1800-0x19ff */ 0x00, 0x78, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1800-0x183f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1840-0x187f */ 0x60, 0x00, 0x00, 0x00, 0x00, 0x02, 0x00, 0x00, /* 0x1880-0x18bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x18c0-0x18ff */ 0x00, 0x00, 0x00, 0x00, 0x87, 0x01, 0x04, 0x0e, /* 0x1900-0x193f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1940-0x197f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1980-0x19bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x19c0-0x19ff */ /* 0x1a00-0x1bff */ 0x00, 0x00, 0x80, 0x09, 0x00, 0x00, 0x00, 0x00, /* 0x1a00-0x1a3f */ 0x00, 0x00, 0x40, 0x7f, 0xe5, 0x1f, 0xf8, 0x9f, /* 0x1a40-0x1a7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xff, 0x7f, /* 0x1a80-0x1abf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1ac0-0x1aff */ 0x0f, 0x00, 0x00, 0x00, 0x00, 0x00, 0xd0, 0x17, /* 0x1b00-0x1b3f */ 0x04, 0x00, 0x00, 0x00, 0x00, 0xf8, 0x0f, 0x00, /* 0x1b40-0x1b7f */ 0x03, 0x00, 0x00, 0x00, 0x3c, 0x3b, 0x00, 0x00, /* 0x1b80-0x1bbf */ 0x00, 0x00, 0x00, 0x00, 0x40, 0xa3, 0x03, 0x00, /* 0x1bc0-0x1bff */ /* 0x1c00-0x1dff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0xf0, 0xcf, 0x00, /* 0x1c00-0x1c3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1c40-0x1c7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1c80-0x1cbf */ 0x00, 0x00, 0xf7, 0xff, 0xfd, 0x21, 0x10, 0x03, /* 0x1cc0-0x1cff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d00-0x1d3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d40-0x1d7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d80-0x1dbf */ 0xff, 0xff, 0xff, 0xff, 0xff, 0xff, 0x3f, 0xf8, /* 0x1dc0-0x1dff */ /* 0x2000-0x21ff */ 0x00, 0xf8, 0x00, 0x00, 0x00, 0x7c, 0x00, 0x00, /* 0x2000-0x203f */ 0x00, 0x00, 0x00, 0x00, 0xdf, 0xff, 0x00, 0x00, /* 0x2040-0x207f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2080-0x20bf */ 0x00, 0x00, 0xff, 0xff, 0xff, 0xff, 0x01, 0x00, /* 0x20c0-0x20ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2100-0x213f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2140-0x217f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2180-0x21bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x21c0-0x21ff */ /* 0x2c00-0x2dff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2c00-0x2c3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2c40-0x2c7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2c80-0x2cbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, 0x03, 0x00, /* 0x2cc0-0x2cff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2d00-0x2d3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, /* 0x2d40-0x2d7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x2d80-0x2dbf */ 0x00, 0x00, 0x00, 0x00, 0xff, 0xff, 0xff, 0xff, /* 0x2dc0-0x2dff */ /* 0x3000-0x31ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x3c, 0x00, 0x00, /* 0x3000-0x303f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x3040-0x307f */ 0x00, 0x00, 0x00, 0x06, 0x00, 0x00, 0x00, 0x00, /* 0x3080-0x30bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x30c0-0x30ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x3100-0x313f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x3140-0x317f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x3180-0x31bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x31c0-0x31ff */ /* 0xa600-0xa7ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa600-0xa63f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, 0xf7, 0x3f, /* 0xa640-0xa67f */ 0x00, 0x00, 0x00, 0xc0, 0x00, 0x00, 0x00, 0x00, /* 0xa680-0xa6bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x03, 0x00, /* 0xa6c0-0xa6ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa700-0xa73f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa740-0xa77f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa780-0xa7bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa7c0-0xa7ff */ /* 0xa800-0xa9ff */ 0x44, 0x08, 0x00, 0x00, 0x60, 0x00, 0x00, 0x00, /* 0xa800-0xa83f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa840-0xa87f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa880-0xa8bf */ 0x30, 0x00, 0x00, 0x00, 0xff, 0xff, 0x03, 0x00, /* 0xa8c0-0xa8ff */ 0x00, 0x00, 0x00, 0x00, 0xc0, 0x3f, 0x00, 0x00, /* 0xa900-0xa93f */ 0x80, 0xff, 0x03, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xa940-0xa97f */ 0x07, 0x00, 0x00, 0x00, 0x00, 0x00, 0xc8, 0x13, /* 0xa980-0xa9bf */ 0x00, 0x00, 0x00, 0x00, 0x20, 0x00, 0x00, 0x00, /* 0xa9c0-0xa9ff */ /* 0xaa00-0xabff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x7e, 0x66, 0x00, /* 0xaa00-0xaa3f */ 0x08, 0x10, 0x00, 0x00, 0x00, 0x00, 0x00, 0x10, /* 0xaa40-0xaa7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x9d, 0xc1, /* 0xaa80-0xaabf */ 0x02, 0x00, 0x00, 0x00, 0x00, 0x30, 0x40, 0x00, /* 0xaac0-0xaaff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xab00-0xab3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xab40-0xab7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xab80-0xabbf */ 0x00, 0x00, 0x00, 0x00, 0x20, 0x21, 0x00, 0x00, /* 0xabc0-0xabff */ /* 0xfa00-0xfbff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfa00-0xfa3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfa40-0xfa7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfa80-0xfabf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfac0-0xfaff */ 0x00, 0x00, 0x00, 0x40, 0x00, 0x00, 0x00, 0x00, /* 0xfb00-0xfb3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfb40-0xfb7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfb80-0xfbbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfbc0-0xfbff */ /* 0xfe00-0xffff */ 0xff, 0xff, 0x00, 0x00, 0xff, 0xff, 0x00, 0x00, /* 0xfe00-0xfe3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfe40-0xfe7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xfe80-0xfebf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, /* 0xfec0-0xfeff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xff00-0xff3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xff40-0xff7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0xff80-0xffbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x0e, /* 0xffc0-0xffff */ /* 0x10000-0x101ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10000-0x1003f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10040-0x1007f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10080-0x100bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x100c0-0x100ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10100-0x1013f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10140-0x1017f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10180-0x101bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x20, /* 0x101c0-0x101ff */ /* 0x10200-0x103ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10200-0x1023f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10240-0x1027f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10280-0x102bf */ 0x00, 0x00, 0x00, 0x00, 0x01, 0x00, 0x00, 0x00, /* 0x102c0-0x102ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10300-0x1033f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xc0, 0x07, /* 0x10340-0x1037f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10380-0x103bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x103c0-0x103ff */ /* 0x10a00-0x10bff */ 0x6e, 0xf0, 0x00, 0x00, 0x00, 0x00, 0x00, 0x87, /* 0x10a00-0x10a3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10a40-0x10a7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10a80-0x10abf */ 0x00, 0x00, 0x00, 0x00, 0x60, 0x00, 0x00, 0x00, /* 0x10ac0-0x10aff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10b00-0x10b3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10b40-0x10b7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10b80-0x10bbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x10bc0-0x10bff */ /* 0x11000-0x111ff */ 0x02, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xff, /* 0x11000-0x1103f */ 0x7f, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, /* 0x11040-0x1107f */ 0x03, 0x00, 0x00, 0x00, 0x00, 0x00, 0x78, 0x26, /* 0x11080-0x110bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x110c0-0x110ff */ 0x07, 0x00, 0x00, 0x00, 0x80, 0xef, 0x1f, 0x00, /* 0x11100-0x1113f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x08, 0x00, /* 0x11140-0x1117f */ 0x03, 0x00, 0x00, 0x00, 0x00, 0x00, 0xc0, 0x7f, /* 0x11180-0x111bf */ 0x00, 0x1c, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x111c0-0x111ff */ /* 0x11200-0x113ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x80, 0xd3, 0x40, /* 0x11200-0x1123f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11240-0x1127f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11280-0x112bf */ 0x00, 0x00, 0x00, 0x80, 0xf8, 0x07, 0x00, 0x00, /* 0x112c0-0x112ff */ 0x03, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x10, /* 0x11300-0x1133f */ 0x01, 0x00, 0x00, 0x00, 0xc0, 0x1f, 0x1f, 0x00, /* 0x11340-0x1137f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11380-0x113bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x113c0-0x113ff */ /* 0x11400-0x115ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xff, /* 0x11400-0x1143f */ 0x5c, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11440-0x1147f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xf8, 0x85, /* 0x11480-0x114bf */ 0x0d, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x114c0-0x114ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11500-0x1153f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11540-0x1157f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x3c, 0xb0, /* 0x11580-0x115bf */ 0x01, 0x00, 0x00, 0x30, 0x00, 0x00, 0x00, 0x00, /* 0x115c0-0x115ff */ /* 0x11600-0x117ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0xf8, 0xa7, /* 0x11600-0x1163f */ 0x01, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11640-0x1167f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x28, 0xbf, 0x00, /* 0x11680-0x116bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x116c0-0x116ff */ 0x00, 0x00, 0x00, 0xe0, 0xbc, 0x0f, 0x00, 0x00, /* 0x11700-0x1173f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11740-0x1177f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11780-0x117bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x117c0-0x117ff */ /* 0x11c00-0x11dff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x7f, 0x3f, /* 0x11c00-0x11c3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11c40-0x11c7f */ 0x00, 0x00, 0xfc, 0xff, 0xff, 0xfc, 0x6d, 0x00, /* 0x11c80-0x11cbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11cc0-0x11cff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11d00-0x11d3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11d40-0x11d7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11d80-0x11dbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x11dc0-0x11dff */ /* 0x16a00-0x16bff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16a00-0x16a3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16a40-0x16a7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16a80-0x16abf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x1f, 0x00, /* 0x16ac0-0x16aff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x7f, 0x00, /* 0x16b00-0x16b3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16b40-0x16b7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16b80-0x16bbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16bc0-0x16bff */ /* 0x16e00-0x16fff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16e00-0x16e3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16e40-0x16e7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16e80-0x16ebf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16ec0-0x16eff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16f00-0x16f3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16f40-0x16f7f */ 0x00, 0x80, 0x07, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16f80-0x16fbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x16fc0-0x16fff */ /* 0x1bc00-0x1bdff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bc00-0x1bc3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bc40-0x1bc7f */ 0x00, 0x00, 0x00, 0x60, 0x0f, 0x00, 0x00, 0x00, /* 0x1bc80-0x1bcbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bcc0-0x1bcff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bd00-0x1bd3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bd40-0x1bd7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bd80-0x1bdbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1bdc0-0x1bdff */ /* 0x1d000-0x1d1ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d000-0x1d03f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d040-0x1d07f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d080-0x1d0bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d0c0-0x1d0ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d100-0x1d13f */ 0x00, 0x00, 0x00, 0x00, 0x80, 0x03, 0xf8, 0xff, /* 0x1d140-0x1d17f */ 0xe7, 0x0f, 0x00, 0x00, 0x00, 0x3c, 0x00, 0x00, /* 0x1d180-0x1d1bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d1c0-0x1d1ff */ /* 0x1d200-0x1d3ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d200-0x1d23f */ 0x1c, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d240-0x1d27f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d280-0x1d2bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d2c0-0x1d2ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d300-0x1d33f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d340-0x1d37f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d380-0x1d3bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1d3c0-0x1d3ff */ /* 0x1da00-0x1dbff */ 0xff, 0xff, 0xff, 0xff, 0xff, 0xff, 0x7f, 0xf8, /* 0x1da00-0x1da3f */ 0xff, 0xff, 0xff, 0xff, 0xff, 0x1f, 0x20, 0x00, /* 0x1da40-0x1da7f */ 0x10, 0x00, 0x00, 0xf8, 0xfe, 0xff, 0x00, 0x00, /* 0x1da80-0x1dabf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1dac0-0x1daff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1db00-0x1db3f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1db40-0x1db7f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1db80-0x1dbbf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1dbc0-0x1dbff */ /* 0x1e000-0x1e1ff */ 0x7f, 0xff, 0xff, 0xf9, 0xdb, 0x07, 0x00, 0x00, /* 0x1e000-0x1e03f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e040-0x1e07f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e080-0x1e0bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e0c0-0x1e0ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e100-0x1e13f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e140-0x1e17f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e180-0x1e1bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e1c0-0x1e1ff */ /* 0x1e800-0x1e9ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e800-0x1e83f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e840-0x1e87f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e880-0x1e8bf */ 0x00, 0x00, 0x7f, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e8c0-0x1e8ff */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e900-0x1e93f */ 0xf0, 0x07, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e940-0x1e97f */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, /* 0x1e980-0x1e9bf */ 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00, 0x00 /* 0x1e9c0-0x1e9ff */ }; static const signed char nonspacing_table_ind[248] = { 0, 1, 2, 3, 4, 5, 6, 7, /* 0x0000-0x0fff */ 8, 9, -1, 10, 11, 12, 13, -1, /* 0x1000-0x1fff */ 14, -1, -1, -1, -1, -1, 15, -1, /* 0x2000-0x2fff */ 16, -1, -1, -1, -1, -1, -1, -1, /* 0x3000-0x3fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x4000-0x4fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x5000-0x5fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x6000-0x6fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x7000-0x7fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x8000-0x8fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x9000-0x9fff */ -1, -1, -1, 17, 18, 19, -1, -1, /* 0xa000-0xafff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0xb000-0xbfff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0xc000-0xcfff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0xd000-0xdfff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0xe000-0xefff */ -1, -1, -1, -1, -1, 20, -1, 21, /* 0xf000-0xffff */ 22, 23, -1, -1, -1, 24, -1, -1, /* 0x10000-0x10fff */ 25, 26, 27, 28, -1, -1, 29, -1, /* 0x11000-0x11fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x12000-0x12fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x13000-0x13fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x14000-0x14fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x15000-0x15fff */ -1, -1, -1, -1, -1, 30, -1, 31, /* 0x16000-0x16fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x17000-0x17fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x18000-0x18fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x19000-0x19fff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x1a000-0x1afff */ -1, -1, -1, -1, -1, -1, 32, -1, /* 0x1b000-0x1bfff */ -1, -1, -1, -1, -1, -1, -1, -1, /* 0x1c000-0x1cfff */ 33, 34, -1, -1, -1, 35, -1, -1, /* 0x1d000-0x1dfff */ 36, -1, -1, -1, 37, -1, -1, -1 /* 0x1e000-0x1efff */ }; /* Determine number of column positions required for UC. */ int uc_width (ucs4_t uc, const char *encoding) { /* Test for non-spacing or control character. */ if ((uc >> 9) < 248) { int ind = nonspacing_table_ind[uc >> 9]; if (ind >= 0) if ((nonspacing_table_data[64*ind + ((uc >> 3) & 63)] >> (uc & 7)) & 1) { if (uc > 0 && uc < 0xa0) return -1; else return 0; } } else if ((uc >> 9) == (0xe0000 >> 9)) { if (uc >= 0xe0100) { if (uc <= 0xe01ef) return 0; } else { if (uc >= 0xe0020 ? uc <= 0xe007f : uc == 0xe0001) return 0; } } /* Test for double-width character. * Generated from "grep '^[^;]\{4,5\};[WF]' EastAsianWidth.txt" * and "grep '^[^;]\{4,5\};[^WF]' EastAsianWidth.txt" */ if (uc >= 0x1100 && ((uc < 0x1160) /* Hangul Jamo */ || (uc >= 0x2329 && uc < 0x232b) /* Angle Brackets */ || (uc >= 0x2e80 && uc < 0xa4d0 /* CJK ... Yi */ && !(uc == 0x303f) && !(uc >= 0x4dc0 && uc < 0x4e00)) || (uc >= 0xac00 && uc < 0xd7a4) /* Hangul Syllables */ || (uc >= 0xf900 && uc < 0xfb00) /* CJK Compatibility Ideographs */ || (uc >= 0xfe10 && uc < 0xfe20) /* Presentation Forms for Vertical */ || (uc >= 0xfe30 && uc < 0xfe70) /* CJK Compatibility Forms */ || (uc >= 0xff00 && uc < 0xff61) /* Fullwidth Forms */ || (uc >= 0xffe0 && uc < 0xffe7) /* Fullwidth Signs */ || (uc >= 0x20000 && uc <= 0x2ffff) /* Supplementary Ideographic Plane */ || (uc >= 0x30000 && uc <= 0x3ffff) /* Tertiary Ideographic Plane */ ) ) return 2; /* In ancient CJK encodings, Cyrillic and most other characters are double-width as well. */ if (uc >= 0x00A1 && uc < 0xFF61 && uc != 0x20A9 && is_cjk_encoding (encoding)) return 2; return 1; } gnuastro-0.5/bootstrapped/lib/glthread/0000755000175000017500000000000013217220465015271 500000000000000gnuastro-0.5/bootstrapped/lib/glthread/threadlib.c0000644000175000017500000000353713217200021017305 00000000000000/* Multithreading primitives. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. */ #include /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # include # if PTHREAD_IN_USE_DETECTION_HARD /* The function to be executed by a dummy thread. */ static void * dummy_thread_func (void *arg) { return arg; } int glthread_in_use (void) { static int tested; static int result; /* 1: linked with -lpthread, 0: only with libc */ if (!tested) { pthread_t thread; if (pthread_create (&thread, NULL, dummy_thread_func, NULL) != 0) /* Thread creation failed. */ result = 0; else { /* Thread creation works. */ void *retval; if (pthread_join (thread, &retval) != 0) abort (); result = 1; } tested = 1; } return result; } # endif #endif /* ========================================================================= */ /* This declaration is solely to ensure that after preprocessing this file is never empty. */ typedef int dummy; gnuastro-0.5/bootstrapped/lib/glthread/lock.c0000644000175000017500000007566013217200021016305 00000000000000/* Locking in multithreaded situations. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ #include #include "glthread/lock.h" /* ========================================================================= */ #if USE_POSIX_THREADS /* -------------------------- gl_lock_t datatype -------------------------- */ /* ------------------------- gl_rwlock_t datatype ------------------------- */ # if HAVE_PTHREAD_RWLOCK && (HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER || (defined PTHREAD_RWLOCK_WRITER_NONRECURSIVE_INITIALIZER_NP && (__GNU_LIBRARY__ > 1))) # ifdef PTHREAD_RWLOCK_INITIALIZER # if !HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER /* glibc with bug https://sourceware.org/bugzilla/show_bug.cgi?id=13701 */ int glthread_rwlock_init_for_glibc (pthread_rwlock_t *lock) { pthread_rwlockattr_t attributes; int err; err = pthread_rwlockattr_init (&attributes); if (err != 0) return err; /* Note: PTHREAD_RWLOCK_PREFER_WRITER_NONRECURSIVE_NP is the only value that causes the writer to be preferred. PTHREAD_RWLOCK_PREFER_WRITER_NP does not do this; see http://man7.org/linux/man-pages/man3/pthread_rwlockattr_setkind_np.3.html */ err = pthread_rwlockattr_setkind_np (&attributes, PTHREAD_RWLOCK_PREFER_WRITER_NONRECURSIVE_NP); if (err == 0) err = pthread_rwlock_init(lock, &attributes); /* pthread_rwlockattr_destroy always returns 0. It cannot influence the return value. */ pthread_rwlockattr_destroy (&attributes); return err; } # endif # else int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_rwlock_init (&lock->rwlock, NULL); if (err != 0) return err; lock->initialized = 1; return 0; } int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) { int err; err = pthread_mutex_lock (&lock->guard); if (err != 0) return err; if (!lock->initialized) { err = glthread_rwlock_init_multithreaded (lock); if (err != 0) { pthread_mutex_unlock (&lock->guard); return err; } } err = pthread_mutex_unlock (&lock->guard); if (err != 0) return err; } return pthread_rwlock_rdlock (&lock->rwlock); } int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) { int err; err = pthread_mutex_lock (&lock->guard); if (err != 0) return err; if (!lock->initialized) { err = glthread_rwlock_init_multithreaded (lock); if (err != 0) { pthread_mutex_unlock (&lock->guard); return err; } } err = pthread_mutex_unlock (&lock->guard); if (err != 0) return err; } return pthread_rwlock_wrlock (&lock->rwlock); } int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) return EINVAL; return pthread_rwlock_unlock (&lock->rwlock); } int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock) { int err; if (!lock->initialized) return EINVAL; err = pthread_rwlock_destroy (&lock->rwlock); if (err != 0) return err; lock->initialized = 0; return 0; } # endif # else int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_init (&lock->lock, NULL); if (err != 0) return err; err = pthread_cond_init (&lock->waiting_readers, NULL); if (err != 0) return err; err = pthread_cond_init (&lock->waiting_writers, NULL); if (err != 0) return err; lock->waiting_writers_count = 0; lock->runcount = 0; return 0; } int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_lock (&lock->lock); if (err != 0) return err; /* Test whether only readers are currently running, and whether the runcount field will not overflow, and whether no writer is waiting. The latter condition is because POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ while (!(lock->runcount + 1 > 0 && lock->waiting_writers_count == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_readers. */ err = pthread_cond_wait (&lock->waiting_readers, &lock->lock); if (err != 0) { pthread_mutex_unlock (&lock->lock); return err; } } lock->runcount++; return pthread_mutex_unlock (&lock->lock); } int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_lock (&lock->lock); if (err != 0) return err; /* Test whether no readers or writers are currently running. */ while (!(lock->runcount == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_writers. */ lock->waiting_writers_count++; err = pthread_cond_wait (&lock->waiting_writers, &lock->lock); if (err != 0) { lock->waiting_writers_count--; pthread_mutex_unlock (&lock->lock); return err; } lock->waiting_writers_count--; } lock->runcount--; /* runcount becomes -1 */ return pthread_mutex_unlock (&lock->lock); } int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_lock (&lock->lock); if (err != 0) return err; if (lock->runcount < 0) { /* Drop a writer lock. */ if (!(lock->runcount == -1)) { pthread_mutex_unlock (&lock->lock); return EINVAL; } lock->runcount = 0; } else { /* Drop a reader lock. */ if (!(lock->runcount > 0)) { pthread_mutex_unlock (&lock->lock); return EINVAL; } lock->runcount--; } if (lock->runcount == 0) { /* POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ if (lock->waiting_writers_count > 0) { /* Wake up one of the waiting writers. */ err = pthread_cond_signal (&lock->waiting_writers); if (err != 0) { pthread_mutex_unlock (&lock->lock); return err; } } else { /* Wake up all waiting readers. */ err = pthread_cond_broadcast (&lock->waiting_readers); if (err != 0) { pthread_mutex_unlock (&lock->lock); return err; } } } return pthread_mutex_unlock (&lock->lock); } int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock) { int err; err = pthread_mutex_destroy (&lock->lock); if (err != 0) return err; err = pthread_cond_destroy (&lock->waiting_readers); if (err != 0) return err; err = pthread_cond_destroy (&lock->waiting_writers); if (err != 0) return err; return 0; } # endif /* --------------------- gl_recursive_lock_t datatype --------------------- */ # if HAVE_PTHREAD_MUTEX_RECURSIVE # if defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER || defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER_NP int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { pthread_mutexattr_t attributes; int err; err = pthread_mutexattr_init (&attributes); if (err != 0) return err; err = pthread_mutexattr_settype (&attributes, PTHREAD_MUTEX_RECURSIVE); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutex_init (lock, &attributes); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutexattr_destroy (&attributes); if (err != 0) return err; return 0; } # else int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { pthread_mutexattr_t attributes; int err; err = pthread_mutexattr_init (&attributes); if (err != 0) return err; err = pthread_mutexattr_settype (&attributes, PTHREAD_MUTEX_RECURSIVE); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutex_init (&lock->recmutex, &attributes); if (err != 0) { pthread_mutexattr_destroy (&attributes); return err; } err = pthread_mutexattr_destroy (&attributes); if (err != 0) return err; lock->initialized = 1; return 0; } int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock) { if (!lock->initialized) { int err; err = pthread_mutex_lock (&lock->guard); if (err != 0) return err; if (!lock->initialized) { err = glthread_recursive_lock_init_multithreaded (lock); if (err != 0) { pthread_mutex_unlock (&lock->guard); return err; } } err = pthread_mutex_unlock (&lock->guard); if (err != 0) return err; } return pthread_mutex_lock (&lock->recmutex); } int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock) { if (!lock->initialized) return EINVAL; return pthread_mutex_unlock (&lock->recmutex); } int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock) { int err; if (!lock->initialized) return EINVAL; err = pthread_mutex_destroy (&lock->recmutex); if (err != 0) return err; lock->initialized = 0; return 0; } # endif # else int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { int err; err = pthread_mutex_init (&lock->mutex, NULL); if (err != 0) return err; lock->owner = (pthread_t) 0; lock->depth = 0; return 0; } int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock) { pthread_t self = pthread_self (); if (lock->owner != self) { int err; err = pthread_mutex_lock (&lock->mutex); if (err != 0) return err; lock->owner = self; } if (++(lock->depth) == 0) /* wraparound? */ { lock->depth--; return EAGAIN; } return 0; } int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != pthread_self ()) return EPERM; if (lock->depth == 0) return EINVAL; if (--(lock->depth) == 0) { lock->owner = (pthread_t) 0; return pthread_mutex_unlock (&lock->mutex); } else return 0; } int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != (pthread_t) 0) return EBUSY; return pthread_mutex_destroy (&lock->mutex); } # endif /* -------------------------- gl_once_t datatype -------------------------- */ static const pthread_once_t fresh_once = PTHREAD_ONCE_INIT; int glthread_once_singlethreaded (pthread_once_t *once_control) { /* We don't know whether pthread_once_t is an integer type, a floating-point type, a pointer type, or a structure type. */ char *firstbyte = (char *)once_control; if (*firstbyte == *(const char *)&fresh_once) { /* First time use of once_control. Invert the first byte. */ *firstbyte = ~ *(const char *)&fresh_once; return 1; } else return 0; } #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ /* -------------------------- gl_lock_t datatype -------------------------- */ /* ------------------------- gl_rwlock_t datatype ------------------------- */ # if !HAVE_PTH_RWLOCK_ACQUIRE_PREFER_WRITER int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock) { if (!pth_mutex_init (&lock->lock)) return errno; if (!pth_cond_init (&lock->waiting_readers)) return errno; if (!pth_cond_init (&lock->waiting_writers)) return errno; lock->waiting_writers_count = 0; lock->runcount = 0; lock->initialized = 1; return 0; } int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) glthread_rwlock_init_multithreaded (lock); if (!pth_mutex_acquire (&lock->lock, 0, NULL)) return errno; /* Test whether only readers are currently running, and whether the runcount field will not overflow, and whether no writer is waiting. The latter condition is because POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ while (!(lock->runcount + 1 > 0 && lock->waiting_writers_count == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_readers. */ if (!pth_cond_await (&lock->waiting_readers, &lock->lock, NULL)) { int err = errno; pth_mutex_release (&lock->lock); return err; } } lock->runcount++; return (!pth_mutex_release (&lock->lock) ? errno : 0); } int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock) { if (!lock->initialized) glthread_rwlock_init_multithreaded (lock); if (!pth_mutex_acquire (&lock->lock, 0, NULL)) return errno; /* Test whether no readers or writers are currently running. */ while (!(lock->runcount == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_writers. */ lock->waiting_writers_count++; if (!pth_cond_await (&lock->waiting_writers, &lock->lock, NULL)) { int err = errno; lock->waiting_writers_count--; pth_mutex_release (&lock->lock); return err; } lock->waiting_writers_count--; } lock->runcount--; /* runcount becomes -1 */ return (!pth_mutex_release (&lock->lock) ? errno : 0); } int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock) { int err; if (!lock->initialized) return EINVAL; if (!pth_mutex_acquire (&lock->lock, 0, NULL)) return errno; if (lock->runcount < 0) { /* Drop a writer lock. */ if (!(lock->runcount == -1)) { pth_mutex_release (&lock->lock); return EINVAL; } lock->runcount = 0; } else { /* Drop a reader lock. */ if (!(lock->runcount > 0)) { pth_mutex_release (&lock->lock); return EINVAL; } lock->runcount--; } if (lock->runcount == 0) { /* POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ if (lock->waiting_writers_count > 0) { /* Wake up one of the waiting writers. */ if (!pth_cond_notify (&lock->waiting_writers, FALSE)) { int err = errno; pth_mutex_release (&lock->lock); return err; } } else { /* Wake up all waiting readers. */ if (!pth_cond_notify (&lock->waiting_readers, TRUE)) { int err = errno; pth_mutex_release (&lock->lock); return err; } } } return (!pth_mutex_release (&lock->lock) ? errno : 0); } int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock) { lock->initialized = 0; return 0; } # endif /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* -------------------------- gl_once_t datatype -------------------------- */ static void glthread_once_call (void *arg) { void (**gl_once_temp_addr) (void) = (void (**) (void)) arg; void (*initfunction) (void) = *gl_once_temp_addr; initfunction (); } int glthread_once_multithreaded (pth_once_t *once_control, void (*initfunction) (void)) { void (*temp) (void) = initfunction; return (!pth_once (once_control, glthread_once_call, &temp) ? errno : 0); } int glthread_once_singlethreaded (pth_once_t *once_control) { /* We know that pth_once_t is an integer type. */ if (*once_control == PTH_ONCE_INIT) { /* First time use of once_control. Invert the marker. */ *once_control = ~ PTH_ONCE_INIT; return 1; } else return 0; } #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ /* -------------------------- gl_lock_t datatype -------------------------- */ /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* --------------------- gl_recursive_lock_t datatype --------------------- */ int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock) { int err; err = mutex_init (&lock->mutex, USYNC_THREAD, NULL); if (err != 0) return err; lock->owner = (thread_t) 0; lock->depth = 0; return 0; } int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock) { thread_t self = thr_self (); if (lock->owner != self) { int err; err = mutex_lock (&lock->mutex); if (err != 0) return err; lock->owner = self; } if (++(lock->depth) == 0) /* wraparound? */ { lock->depth--; return EAGAIN; } return 0; } int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != thr_self ()) return EPERM; if (lock->depth == 0) return EINVAL; if (--(lock->depth) == 0) { lock->owner = (thread_t) 0; return mutex_unlock (&lock->mutex); } else return 0; } int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock) { if (lock->owner != (thread_t) 0) return EBUSY; return mutex_destroy (&lock->mutex); } /* -------------------------- gl_once_t datatype -------------------------- */ int glthread_once_multithreaded (gl_once_t *once_control, void (*initfunction) (void)) { if (!once_control->inited) { int err; /* Use the mutex to guarantee that if another thread is already calling the initfunction, this thread waits until it's finished. */ err = mutex_lock (&once_control->mutex); if (err != 0) return err; if (!once_control->inited) { once_control->inited = 1; initfunction (); } return mutex_unlock (&once_control->mutex); } else return 0; } int glthread_once_singlethreaded (gl_once_t *once_control) { /* We know that gl_once_t contains an integer type. */ if (!once_control->inited) { /* First time use of once_control. Invert the marker. */ once_control->inited = ~ 0; return 1; } else return 0; } #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS /* -------------------------- gl_lock_t datatype -------------------------- */ void glthread_lock_init_func (gl_lock_t *lock) { InitializeCriticalSection (&lock->lock); lock->guard.done = 1; } int glthread_lock_lock_func (gl_lock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_lock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } EnterCriticalSection (&lock->lock); return 0; } int glthread_lock_unlock_func (gl_lock_t *lock) { if (!lock->guard.done) return EINVAL; LeaveCriticalSection (&lock->lock); return 0; } int glthread_lock_destroy_func (gl_lock_t *lock) { if (!lock->guard.done) return EINVAL; DeleteCriticalSection (&lock->lock); lock->guard.done = 0; return 0; } /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* In this file, the waitqueues are implemented as circular arrays. */ #define gl_waitqueue_t gl_carray_waitqueue_t static void gl_waitqueue_init (gl_waitqueue_t *wq) { wq->array = NULL; wq->count = 0; wq->alloc = 0; wq->offset = 0; } /* Enqueues the current thread, represented by an event, in a wait queue. Returns INVALID_HANDLE_VALUE if an allocation failure occurs. */ static HANDLE gl_waitqueue_add (gl_waitqueue_t *wq) { HANDLE event; unsigned int index; if (wq->count == wq->alloc) { unsigned int new_alloc = 2 * wq->alloc + 1; HANDLE *new_array = (HANDLE *) realloc (wq->array, new_alloc * sizeof (HANDLE)); if (new_array == NULL) /* No more memory. */ return INVALID_HANDLE_VALUE; /* Now is a good opportunity to rotate the array so that its contents starts at offset 0. */ if (wq->offset > 0) { unsigned int old_count = wq->count; unsigned int old_alloc = wq->alloc; unsigned int old_offset = wq->offset; unsigned int i; if (old_offset + old_count > old_alloc) { unsigned int limit = old_offset + old_count - old_alloc; for (i = 0; i < limit; i++) new_array[old_alloc + i] = new_array[i]; } for (i = 0; i < old_count; i++) new_array[i] = new_array[old_offset + i]; wq->offset = 0; } wq->array = new_array; wq->alloc = new_alloc; } /* Whether the created event is a manual-reset one or an auto-reset one, does not matter, since we will wait on it only once. */ event = CreateEvent (NULL, TRUE, FALSE, NULL); if (event == INVALID_HANDLE_VALUE) /* No way to allocate an event. */ return INVALID_HANDLE_VALUE; index = wq->offset + wq->count; if (index >= wq->alloc) index -= wq->alloc; wq->array[index] = event; wq->count++; return event; } /* Notifies the first thread from a wait queue and dequeues it. */ static void gl_waitqueue_notify_first (gl_waitqueue_t *wq) { SetEvent (wq->array[wq->offset + 0]); wq->offset++; wq->count--; if (wq->count == 0 || wq->offset == wq->alloc) wq->offset = 0; } /* Notifies all threads from a wait queue and dequeues them all. */ static void gl_waitqueue_notify_all (gl_waitqueue_t *wq) { unsigned int i; for (i = 0; i < wq->count; i++) { unsigned int index = wq->offset + i; if (index >= wq->alloc) index -= wq->alloc; SetEvent (wq->array[index]); } wq->count = 0; wq->offset = 0; } void glthread_rwlock_init_func (gl_rwlock_t *lock) { InitializeCriticalSection (&lock->lock); gl_waitqueue_init (&lock->waiting_readers); gl_waitqueue_init (&lock->waiting_writers); lock->runcount = 0; lock->guard.done = 1; } int glthread_rwlock_rdlock_func (gl_rwlock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_rwlock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } EnterCriticalSection (&lock->lock); /* Test whether only readers are currently running, and whether the runcount field will not overflow, and whether no writer is waiting. The latter condition is because POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ if (!(lock->runcount + 1 > 0 && lock->waiting_writers.count == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_readers. */ HANDLE event = gl_waitqueue_add (&lock->waiting_readers); if (event != INVALID_HANDLE_VALUE) { DWORD result; LeaveCriticalSection (&lock->lock); /* Wait until another thread signals this event. */ result = WaitForSingleObject (event, INFINITE); if (result == WAIT_FAILED || result == WAIT_TIMEOUT) abort (); CloseHandle (event); /* The thread which signalled the event already did the bookkeeping: removed us from the waiting_readers, incremented lock->runcount. */ if (!(lock->runcount > 0)) abort (); return 0; } else { /* Allocation failure. Weird. */ do { LeaveCriticalSection (&lock->lock); Sleep (1); EnterCriticalSection (&lock->lock); } while (!(lock->runcount + 1 > 0)); } } lock->runcount++; LeaveCriticalSection (&lock->lock); return 0; } int glthread_rwlock_wrlock_func (gl_rwlock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_rwlock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } EnterCriticalSection (&lock->lock); /* Test whether no readers or writers are currently running. */ if (!(lock->runcount == 0)) { /* This thread has to wait for a while. Enqueue it among the waiting_writers. */ HANDLE event = gl_waitqueue_add (&lock->waiting_writers); if (event != INVALID_HANDLE_VALUE) { DWORD result; LeaveCriticalSection (&lock->lock); /* Wait until another thread signals this event. */ result = WaitForSingleObject (event, INFINITE); if (result == WAIT_FAILED || result == WAIT_TIMEOUT) abort (); CloseHandle (event); /* The thread which signalled the event already did the bookkeeping: removed us from the waiting_writers, set lock->runcount = -1. */ if (!(lock->runcount == -1)) abort (); return 0; } else { /* Allocation failure. Weird. */ do { LeaveCriticalSection (&lock->lock); Sleep (1); EnterCriticalSection (&lock->lock); } while (!(lock->runcount == 0)); } } lock->runcount--; /* runcount becomes -1 */ LeaveCriticalSection (&lock->lock); return 0; } int glthread_rwlock_unlock_func (gl_rwlock_t *lock) { if (!lock->guard.done) return EINVAL; EnterCriticalSection (&lock->lock); if (lock->runcount < 0) { /* Drop a writer lock. */ if (!(lock->runcount == -1)) abort (); lock->runcount = 0; } else { /* Drop a reader lock. */ if (!(lock->runcount > 0)) { LeaveCriticalSection (&lock->lock); return EPERM; } lock->runcount--; } if (lock->runcount == 0) { /* POSIX recommends that "write locks shall take precedence over read locks", to avoid "writer starvation". */ if (lock->waiting_writers.count > 0) { /* Wake up one of the waiting writers. */ lock->runcount--; gl_waitqueue_notify_first (&lock->waiting_writers); } else { /* Wake up all waiting readers. */ lock->runcount += lock->waiting_readers.count; gl_waitqueue_notify_all (&lock->waiting_readers); } } LeaveCriticalSection (&lock->lock); return 0; } int glthread_rwlock_destroy_func (gl_rwlock_t *lock) { if (!lock->guard.done) return EINVAL; if (lock->runcount != 0) return EBUSY; DeleteCriticalSection (&lock->lock); if (lock->waiting_readers.array != NULL) free (lock->waiting_readers.array); if (lock->waiting_writers.array != NULL) free (lock->waiting_writers.array); lock->guard.done = 0; return 0; } /* --------------------- gl_recursive_lock_t datatype --------------------- */ void glthread_recursive_lock_init_func (gl_recursive_lock_t *lock) { lock->owner = 0; lock->depth = 0; InitializeCriticalSection (&lock->lock); lock->guard.done = 1; } int glthread_recursive_lock_lock_func (gl_recursive_lock_t *lock) { if (!lock->guard.done) { if (InterlockedIncrement (&lock->guard.started) == 0) /* This thread is the first one to need this lock. Initialize it. */ glthread_recursive_lock_init (lock); else /* Yield the CPU while waiting for another thread to finish initializing this lock. */ while (!lock->guard.done) Sleep (0); } { DWORD self = GetCurrentThreadId (); if (lock->owner != self) { EnterCriticalSection (&lock->lock); lock->owner = self; } if (++(lock->depth) == 0) /* wraparound? */ { lock->depth--; return EAGAIN; } } return 0; } int glthread_recursive_lock_unlock_func (gl_recursive_lock_t *lock) { if (lock->owner != GetCurrentThreadId ()) return EPERM; if (lock->depth == 0) return EINVAL; if (--(lock->depth) == 0) { lock->owner = 0; LeaveCriticalSection (&lock->lock); } return 0; } int glthread_recursive_lock_destroy_func (gl_recursive_lock_t *lock) { if (lock->owner != 0) return EBUSY; DeleteCriticalSection (&lock->lock); lock->guard.done = 0; return 0; } /* -------------------------- gl_once_t datatype -------------------------- */ void glthread_once_func (gl_once_t *once_control, void (*initfunction) (void)) { if (once_control->inited <= 0) { if (InterlockedIncrement (&once_control->started) == 0) { /* This thread is the first one to come to this once_control. */ InitializeCriticalSection (&once_control->lock); EnterCriticalSection (&once_control->lock); once_control->inited = 0; initfunction (); once_control->inited = 1; LeaveCriticalSection (&once_control->lock); } else { /* Undo last operation. */ InterlockedDecrement (&once_control->started); /* Some other thread has already started the initialization. Yield the CPU while waiting for the other thread to finish initializing and taking the lock. */ while (once_control->inited < 0) Sleep (0); if (once_control->inited <= 0) { /* Take the lock. This blocks until the other thread has finished calling the initfunction. */ EnterCriticalSection (&once_control->lock); LeaveCriticalSection (&once_control->lock); if (!(once_control->inited > 0)) abort (); } } } } #endif /* ========================================================================= */ gnuastro-0.5/bootstrapped/lib/glthread/lock.h0000644000175000017500000011346013217200021016301 00000000000000/* Locking in multithreaded situations. Copyright (C) 2005-2017 Free Software Foundation, Inc. This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 3, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, see . */ /* Written by Bruno Haible , 2005. Based on GCC's gthr-posix.h, gthr-posix95.h, gthr-solaris.h, gthr-win32.h. */ /* This file contains locking primitives for use with a given thread library. It does not contain primitives for creating threads or for other synchronization primitives. Normal (non-recursive) locks: Type: gl_lock_t Declaration: gl_lock_define(extern, name) Initializer: gl_lock_define_initialized(, name) Initialization: gl_lock_init (name); Taking the lock: gl_lock_lock (name); Releasing the lock: gl_lock_unlock (name); De-initialization: gl_lock_destroy (name); Equivalent functions with control of error handling: Initialization: err = glthread_lock_init (&name); Taking the lock: err = glthread_lock_lock (&name); Releasing the lock: err = glthread_lock_unlock (&name); De-initialization: err = glthread_lock_destroy (&name); Read-Write (non-recursive) locks: Type: gl_rwlock_t Declaration: gl_rwlock_define(extern, name) Initializer: gl_rwlock_define_initialized(, name) Initialization: gl_rwlock_init (name); Taking the lock: gl_rwlock_rdlock (name); gl_rwlock_wrlock (name); Releasing the lock: gl_rwlock_unlock (name); De-initialization: gl_rwlock_destroy (name); Equivalent functions with control of error handling: Initialization: err = glthread_rwlock_init (&name); Taking the lock: err = glthread_rwlock_rdlock (&name); err = glthread_rwlock_wrlock (&name); Releasing the lock: err = glthread_rwlock_unlock (&name); De-initialization: err = glthread_rwlock_destroy (&name); Recursive locks: Type: gl_recursive_lock_t Declaration: gl_recursive_lock_define(extern, name) Initializer: gl_recursive_lock_define_initialized(, name) Initialization: gl_recursive_lock_init (name); Taking the lock: gl_recursive_lock_lock (name); Releasing the lock: gl_recursive_lock_unlock (name); De-initialization: gl_recursive_lock_destroy (name); Equivalent functions with control of error handling: Initialization: err = glthread_recursive_lock_init (&name); Taking the lock: err = glthread_recursive_lock_lock (&name); Releasing the lock: err = glthread_recursive_lock_unlock (&name); De-initialization: err = glthread_recursive_lock_destroy (&name); Once-only execution: Type: gl_once_t Initializer: gl_once_define(extern, name) Execution: gl_once (name, initfunction); Equivalent functions with control of error handling: Execution: err = glthread_once (&name, initfunction); */ #ifndef _LOCK_H #define _LOCK_H #include #include /* ========================================================================= */ #if USE_POSIX_THREADS /* Use the POSIX threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if PTHREAD_IN_USE_DETECTION_HARD /* The pthread_in_use() detection needs to be done at runtime. */ # define pthread_in_use() \ glthread_in_use () extern int glthread_in_use (void); # endif # if USE_POSIX_THREADS_WEAK /* Use weak references to the POSIX threads library. */ /* Weak references avoid dragging in external libraries if the other parts of the program don't use them. Here we use them, because we don't want every program that uses libintl to depend on libpthread. This assumes that libpthread would not be loaded after libintl; i.e. if libintl is loaded first, by an executable that does not depend on libpthread, and then a module is dynamically loaded that depends on libpthread, libintl will not be multithread-safe. */ /* The way to test at runtime whether libpthread is present is to test whether a function pointer's value, such as &pthread_mutex_init, is non-NULL. However, some versions of GCC have a bug through which, in PIC mode, &foo != NULL always evaluates to true if there is a direct call to foo(...) in the same function. To avoid this, we test the address of a function in libpthread that we don't use. */ # pragma weak pthread_mutex_init # pragma weak pthread_mutex_lock # pragma weak pthread_mutex_unlock # pragma weak pthread_mutex_destroy # pragma weak pthread_rwlock_init # pragma weak pthread_rwlock_rdlock # pragma weak pthread_rwlock_wrlock # pragma weak pthread_rwlock_unlock # pragma weak pthread_rwlock_destroy # pragma weak pthread_once # pragma weak pthread_cond_init # pragma weak pthread_cond_wait # pragma weak pthread_cond_signal # pragma weak pthread_cond_broadcast # pragma weak pthread_cond_destroy # pragma weak pthread_mutexattr_init # pragma weak pthread_mutexattr_settype # pragma weak pthread_mutexattr_destroy # pragma weak pthread_rwlockattr_init # if __GNU_LIBRARY__ > 1 # pragma weak pthread_rwlockattr_setkind_np # endif # pragma weak pthread_rwlockattr_destroy # ifndef pthread_self # pragma weak pthread_self # endif # if !PTHREAD_IN_USE_DETECTION_HARD # pragma weak pthread_cancel # define pthread_in_use() (pthread_cancel != NULL) # endif # else # if !PTHREAD_IN_USE_DETECTION_HARD # define pthread_in_use() 1 # endif # endif /* -------------------------- gl_lock_t datatype -------------------------- */ typedef pthread_mutex_t gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME = gl_lock_initializer; # define gl_lock_initializer \ PTHREAD_MUTEX_INITIALIZER # define glthread_lock_init(LOCK) \ (pthread_in_use () ? pthread_mutex_init (LOCK, NULL) : 0) # define glthread_lock_lock(LOCK) \ (pthread_in_use () ? pthread_mutex_lock (LOCK) : 0) # define glthread_lock_unlock(LOCK) \ (pthread_in_use () ? pthread_mutex_unlock (LOCK) : 0) # define glthread_lock_destroy(LOCK) \ (pthread_in_use () ? pthread_mutex_destroy (LOCK) : 0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ # if HAVE_PTHREAD_RWLOCK && (HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER || (defined PTHREAD_RWLOCK_WRITER_NONRECURSIVE_INITIALIZER_NP && (__GNU_LIBRARY__ > 1))) # ifdef PTHREAD_RWLOCK_INITIALIZER typedef pthread_rwlock_t gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pthread_rwlock_t NAME = gl_rwlock_initializer; # if HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER # define gl_rwlock_initializer \ PTHREAD_RWLOCK_INITIALIZER # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? pthread_rwlock_init (LOCK, NULL) : 0) # else /* glibc with bug https://sourceware.org/bugzilla/show_bug.cgi?id=13701 */ # define gl_rwlock_initializer \ PTHREAD_RWLOCK_WRITER_NONRECURSIVE_INITIALIZER_NP # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? glthread_rwlock_init_for_glibc (LOCK) : 0) extern int glthread_rwlock_init_for_glibc (pthread_rwlock_t *lock); # endif # define glthread_rwlock_rdlock(LOCK) \ (pthread_in_use () ? pthread_rwlock_rdlock (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pthread_in_use () ? pthread_rwlock_wrlock (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pthread_in_use () ? pthread_rwlock_unlock (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pthread_in_use () ? pthread_rwlock_destroy (LOCK) : 0) # else typedef struct { int initialized; pthread_mutex_t guard; /* protects the initialization */ pthread_rwlock_t rwlock; /* read-write lock */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { 0, PTHREAD_MUTEX_INITIALIZER } # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? glthread_rwlock_init_multithreaded (LOCK) : 0) # define glthread_rwlock_rdlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_rdlock_multithreaded (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_wrlock_multithreaded (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_unlock_multithreaded (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pthread_in_use () ? glthread_rwlock_destroy_multithreaded (LOCK) : 0) extern int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock); # endif # else typedef struct { pthread_mutex_t lock; /* protects the remaining fields */ pthread_cond_t waiting_readers; /* waiting readers */ pthread_cond_t waiting_writers; /* waiting writers */ unsigned int waiting_writers_count; /* number of waiting writers */ int runcount; /* number of readers running, or -1 when a writer runs */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { PTHREAD_MUTEX_INITIALIZER, PTHREAD_COND_INITIALIZER, PTHREAD_COND_INITIALIZER, 0, 0 } # define glthread_rwlock_init(LOCK) \ (pthread_in_use () ? glthread_rwlock_init_multithreaded (LOCK) : 0) # define glthread_rwlock_rdlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_rdlock_multithreaded (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_wrlock_multithreaded (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pthread_in_use () ? glthread_rwlock_unlock_multithreaded (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pthread_in_use () ? glthread_rwlock_destroy_multithreaded (LOCK) : 0) extern int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock); # endif /* --------------------- gl_recursive_lock_t datatype --------------------- */ # if HAVE_PTHREAD_MUTEX_RECURSIVE # if defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER || defined PTHREAD_RECURSIVE_MUTEX_INITIALIZER_NP typedef pthread_mutex_t gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pthread_mutex_t NAME = gl_recursive_lock_initializer; # ifdef PTHREAD_RECURSIVE_MUTEX_INITIALIZER # define gl_recursive_lock_initializer \ PTHREAD_RECURSIVE_MUTEX_INITIALIZER # else # define gl_recursive_lock_initializer \ PTHREAD_RECURSIVE_MUTEX_INITIALIZER_NP # endif # define glthread_recursive_lock_init(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (pthread_in_use () ? pthread_mutex_lock (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pthread_in_use () ? pthread_mutex_unlock (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (pthread_in_use () ? pthread_mutex_destroy (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); # else typedef struct { pthread_mutex_t recmutex; /* recursive mutex */ pthread_mutex_t guard; /* protects the initialization */ int initialized; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { PTHREAD_MUTEX_INITIALIZER, PTHREAD_MUTEX_INITIALIZER, 0 } # define glthread_recursive_lock_init(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_lock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_unlock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_destroy_multithreaded (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock); # endif # else /* Old versions of POSIX threads on Solaris did not have recursive locks. We have to implement them ourselves. */ typedef struct { pthread_mutex_t mutex; pthread_t owner; unsigned long depth; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { PTHREAD_MUTEX_INITIALIZER, (pthread_t) 0, 0 } # define glthread_recursive_lock_init(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_lock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_unlock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (pthread_in_use () ? glthread_recursive_lock_destroy_multithreaded (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock); # endif /* -------------------------- gl_once_t datatype -------------------------- */ typedef pthread_once_t gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS pthread_once_t NAME = PTHREAD_ONCE_INIT; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (pthread_in_use () \ ? pthread_once (ONCE_CONTROL, INITFUNCTION) \ : (glthread_once_singlethreaded (ONCE_CONTROL) ? (INITFUNCTION (), 0) : 0)) extern int glthread_once_singlethreaded (pthread_once_t *once_control); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_PTH_THREADS /* Use the GNU Pth threads library. */ # include # ifdef __cplusplus extern "C" { # endif # if USE_PTH_THREADS_WEAK /* Use weak references to the GNU Pth threads library. */ # pragma weak pth_mutex_init # pragma weak pth_mutex_acquire # pragma weak pth_mutex_release # pragma weak pth_rwlock_init # pragma weak pth_rwlock_acquire # pragma weak pth_rwlock_release # pragma weak pth_once # pragma weak pth_cancel # define pth_in_use() (pth_cancel != NULL) # else # define pth_in_use() 1 # endif /* -------------------------- gl_lock_t datatype -------------------------- */ typedef pth_mutex_t gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME = gl_lock_initializer; # define gl_lock_initializer \ PTH_MUTEX_INIT # define glthread_lock_init(LOCK) \ (pth_in_use () && !pth_mutex_init (LOCK) ? errno : 0) # define glthread_lock_lock(LOCK) \ (pth_in_use () && !pth_mutex_acquire (LOCK, 0, NULL) ? errno : 0) # define glthread_lock_unlock(LOCK) \ (pth_in_use () && !pth_mutex_release (LOCK) ? errno : 0) # define glthread_lock_destroy(LOCK) \ ((void)(LOCK), 0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* Pth pth_rwlock_acquire always prefers readers. No autoconf test so far. */ # if HAVE_PTH_RWLOCK_ACQUIRE_PREFER_WRITER typedef pth_rwlock_t gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS pth_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pth_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ PTH_RWLOCK_INIT # define glthread_rwlock_init(LOCK) \ (pth_in_use () && !pth_rwlock_init (LOCK) ? errno : 0) # define glthread_rwlock_rdlock(LOCK) \ (pth_in_use () && !pth_rwlock_acquire (LOCK, PTH_RWLOCK_RD, 0, NULL) ? errno : 0) # define glthread_rwlock_wrlock(LOCK) \ (pth_in_use () && !pth_rwlock_acquire (LOCK, PTH_RWLOCK_RW, 0, NULL) ? errno : 0) # define glthread_rwlock_unlock(LOCK) \ (pth_in_use () && !pth_rwlock_release (LOCK) ? errno : 0) # define glthread_rwlock_destroy(LOCK) \ ((void)(LOCK), 0) # else typedef struct { int initialized; pth_mutex_t lock; /* protects the remaining fields */ pth_cond_t waiting_readers; /* waiting readers */ pth_cond_t waiting_writers; /* waiting writers */ unsigned int waiting_writers_count; /* number of waiting writers */ int runcount; /* number of readers running, or -1 when a writer runs */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { 0 } # define glthread_rwlock_init(LOCK) \ (pth_in_use () ? glthread_rwlock_init_multithreaded (LOCK) : 0) # define glthread_rwlock_rdlock(LOCK) \ (pth_in_use () ? glthread_rwlock_rdlock_multithreaded (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (pth_in_use () ? glthread_rwlock_wrlock_multithreaded (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (pth_in_use () ? glthread_rwlock_unlock_multithreaded (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (pth_in_use () ? glthread_rwlock_destroy_multithreaded (LOCK) : 0) extern int glthread_rwlock_init_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_multithreaded (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_multithreaded (gl_rwlock_t *lock); # endif /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* In Pth, mutexes are recursive by default. */ typedef pth_mutex_t gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS pth_mutex_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ PTH_MUTEX_INIT # define glthread_recursive_lock_init(LOCK) \ (pth_in_use () && !pth_mutex_init (LOCK) ? errno : 0) # define glthread_recursive_lock_lock(LOCK) \ (pth_in_use () && !pth_mutex_acquire (LOCK, 0, NULL) ? errno : 0) # define glthread_recursive_lock_unlock(LOCK) \ (pth_in_use () && !pth_mutex_release (LOCK) ? errno : 0) # define glthread_recursive_lock_destroy(LOCK) \ ((void)(LOCK), 0) /* -------------------------- gl_once_t datatype -------------------------- */ typedef pth_once_t gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS pth_once_t NAME = PTH_ONCE_INIT; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (pth_in_use () \ ? glthread_once_multithreaded (ONCE_CONTROL, INITFUNCTION) \ : (glthread_once_singlethreaded (ONCE_CONTROL) ? (INITFUNCTION (), 0) : 0)) extern int glthread_once_multithreaded (pth_once_t *once_control, void (*initfunction) (void)); extern int glthread_once_singlethreaded (pth_once_t *once_control); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_SOLARIS_THREADS /* Use the old Solaris threads library. */ # include # include # ifdef __cplusplus extern "C" { # endif # if USE_SOLARIS_THREADS_WEAK /* Use weak references to the old Solaris threads library. */ # pragma weak mutex_init # pragma weak mutex_lock # pragma weak mutex_unlock # pragma weak mutex_destroy # pragma weak rwlock_init # pragma weak rw_rdlock # pragma weak rw_wrlock # pragma weak rw_unlock # pragma weak rwlock_destroy # pragma weak thr_self # pragma weak thr_suspend # define thread_in_use() (thr_suspend != NULL) # else # define thread_in_use() 1 # endif /* -------------------------- gl_lock_t datatype -------------------------- */ typedef mutex_t gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS mutex_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS mutex_t NAME = gl_lock_initializer; # define gl_lock_initializer \ DEFAULTMUTEX # define glthread_lock_init(LOCK) \ (thread_in_use () ? mutex_init (LOCK, USYNC_THREAD, NULL) : 0) # define glthread_lock_lock(LOCK) \ (thread_in_use () ? mutex_lock (LOCK) : 0) # define glthread_lock_unlock(LOCK) \ (thread_in_use () ? mutex_unlock (LOCK) : 0) # define glthread_lock_destroy(LOCK) \ (thread_in_use () ? mutex_destroy (LOCK) : 0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ typedef rwlock_t gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ DEFAULTRWLOCK # define glthread_rwlock_init(LOCK) \ (thread_in_use () ? rwlock_init (LOCK, USYNC_THREAD, NULL) : 0) # define glthread_rwlock_rdlock(LOCK) \ (thread_in_use () ? rw_rdlock (LOCK) : 0) # define glthread_rwlock_wrlock(LOCK) \ (thread_in_use () ? rw_wrlock (LOCK) : 0) # define glthread_rwlock_unlock(LOCK) \ (thread_in_use () ? rw_unlock (LOCK) : 0) # define glthread_rwlock_destroy(LOCK) \ (thread_in_use () ? rwlock_destroy (LOCK) : 0) /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* Old Solaris threads did not have recursive locks. We have to implement them ourselves. */ typedef struct { mutex_t mutex; thread_t owner; unsigned long depth; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { DEFAULTMUTEX, (thread_t) 0, 0 } # define glthread_recursive_lock_init(LOCK) \ (thread_in_use () ? glthread_recursive_lock_init_multithreaded (LOCK) : 0) # define glthread_recursive_lock_lock(LOCK) \ (thread_in_use () ? glthread_recursive_lock_lock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_unlock(LOCK) \ (thread_in_use () ? glthread_recursive_lock_unlock_multithreaded (LOCK) : 0) # define glthread_recursive_lock_destroy(LOCK) \ (thread_in_use () ? glthread_recursive_lock_destroy_multithreaded (LOCK) : 0) extern int glthread_recursive_lock_init_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_multithreaded (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_multithreaded (gl_recursive_lock_t *lock); /* -------------------------- gl_once_t datatype -------------------------- */ typedef struct { volatile int inited; mutex_t mutex; } gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS gl_once_t NAME = { 0, DEFAULTMUTEX }; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (thread_in_use () \ ? glthread_once_multithreaded (ONCE_CONTROL, INITFUNCTION) \ : (glthread_once_singlethreaded (ONCE_CONTROL) ? (INITFUNCTION (), 0) : 0)) extern int glthread_once_multithreaded (gl_once_t *once_control, void (*initfunction) (void)); extern int glthread_once_singlethreaded (gl_once_t *once_control); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if USE_WINDOWS_THREADS # define WIN32_LEAN_AND_MEAN /* avoid including junk */ # include # ifdef __cplusplus extern "C" { # endif /* We can use CRITICAL_SECTION directly, rather than the native Windows Event, Mutex, Semaphore types, because - we need only to synchronize inside a single process (address space), not inter-process locking, - we don't need to support trylock operations. (TryEnterCriticalSection does not work on Windows 95/98/ME. Packages that need trylock usually define their own mutex type.) */ /* There is no way to statically initialize a CRITICAL_SECTION. It needs to be done lazily, once only. For this we need spinlocks. */ typedef struct { volatile int done; volatile long started; } gl_spinlock_t; /* -------------------------- gl_lock_t datatype -------------------------- */ typedef struct { gl_spinlock_t guard; /* protects the initialization */ CRITICAL_SECTION lock; } gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_lock_t NAME; # define gl_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_lock_t NAME = gl_lock_initializer; # define gl_lock_initializer \ { { 0, -1 } } # define glthread_lock_init(LOCK) \ (glthread_lock_init_func (LOCK), 0) # define glthread_lock_lock(LOCK) \ glthread_lock_lock_func (LOCK) # define glthread_lock_unlock(LOCK) \ glthread_lock_unlock_func (LOCK) # define glthread_lock_destroy(LOCK) \ glthread_lock_destroy_func (LOCK) extern void glthread_lock_init_func (gl_lock_t *lock); extern int glthread_lock_lock_func (gl_lock_t *lock); extern int glthread_lock_unlock_func (gl_lock_t *lock); extern int glthread_lock_destroy_func (gl_lock_t *lock); /* ------------------------- gl_rwlock_t datatype ------------------------- */ /* It is impossible to implement read-write locks using plain locks, without introducing an extra thread dedicated to managing read-write locks. Therefore here we need to use the low-level Event type. */ typedef struct { HANDLE *array; /* array of waiting threads, each represented by an event */ unsigned int count; /* number of waiting threads */ unsigned int alloc; /* length of allocated array */ unsigned int offset; /* index of first waiting thread in array */ } gl_carray_waitqueue_t; typedef struct { gl_spinlock_t guard; /* protects the initialization */ CRITICAL_SECTION lock; /* protects the remaining fields */ gl_carray_waitqueue_t waiting_readers; /* waiting readers */ gl_carray_waitqueue_t waiting_writers; /* waiting writers */ int runcount; /* number of readers running, or -1 when a writer runs */ } gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME; # define gl_rwlock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_rwlock_t NAME = gl_rwlock_initializer; # define gl_rwlock_initializer \ { { 0, -1 } } # define glthread_rwlock_init(LOCK) \ (glthread_rwlock_init_func (LOCK), 0) # define glthread_rwlock_rdlock(LOCK) \ glthread_rwlock_rdlock_func (LOCK) # define glthread_rwlock_wrlock(LOCK) \ glthread_rwlock_wrlock_func (LOCK) # define glthread_rwlock_unlock(LOCK) \ glthread_rwlock_unlock_func (LOCK) # define glthread_rwlock_destroy(LOCK) \ glthread_rwlock_destroy_func (LOCK) extern void glthread_rwlock_init_func (gl_rwlock_t *lock); extern int glthread_rwlock_rdlock_func (gl_rwlock_t *lock); extern int glthread_rwlock_wrlock_func (gl_rwlock_t *lock); extern int glthread_rwlock_unlock_func (gl_rwlock_t *lock); extern int glthread_rwlock_destroy_func (gl_rwlock_t *lock); /* --------------------- gl_recursive_lock_t datatype --------------------- */ /* The native Windows documentation says that CRITICAL_SECTION already implements a recursive lock. But we need not rely on it: It's easy to implement a recursive lock without this assumption. */ typedef struct { gl_spinlock_t guard; /* protects the initialization */ DWORD owner; unsigned long depth; CRITICAL_SECTION lock; } gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME; # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) \ STORAGECLASS gl_recursive_lock_t NAME = gl_recursive_lock_initializer; # define gl_recursive_lock_initializer \ { { 0, -1 }, 0, 0 } # define glthread_recursive_lock_init(LOCK) \ (glthread_recursive_lock_init_func (LOCK), 0) # define glthread_recursive_lock_lock(LOCK) \ glthread_recursive_lock_lock_func (LOCK) # define glthread_recursive_lock_unlock(LOCK) \ glthread_recursive_lock_unlock_func (LOCK) # define glthread_recursive_lock_destroy(LOCK) \ glthread_recursive_lock_destroy_func (LOCK) extern void glthread_recursive_lock_init_func (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_lock_func (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_unlock_func (gl_recursive_lock_t *lock); extern int glthread_recursive_lock_destroy_func (gl_recursive_lock_t *lock); /* -------------------------- gl_once_t datatype -------------------------- */ typedef struct { volatile int inited; volatile long started; CRITICAL_SECTION lock; } gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS gl_once_t NAME = { -1, -1 }; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (glthread_once_func (ONCE_CONTROL, INITFUNCTION), 0) extern void glthread_once_func (gl_once_t *once_control, void (*initfunction) (void)); # ifdef __cplusplus } # endif #endif /* ========================================================================= */ #if !(USE_POSIX_THREADS || USE_PTH_THREADS || USE_SOLARIS_THREADS || USE_WINDOWS_THREADS) /* Provide dummy implementation if threads are not supported. */ /* -------------------------- gl_lock_t datatype -------------------------- */ typedef int gl_lock_t; # define gl_lock_define(STORAGECLASS, NAME) # define gl_lock_define_initialized(STORAGECLASS, NAME) # define glthread_lock_init(NAME) 0 # define glthread_lock_lock(NAME) 0 # define glthread_lock_unlock(NAME) 0 # define glthread_lock_destroy(NAME) 0 /* ------------------------- gl_rwlock_t datatype ------------------------- */ typedef int gl_rwlock_t; # define gl_rwlock_define(STORAGECLASS, NAME) # define gl_rwlock_define_initialized(STORAGECLASS, NAME) # define glthread_rwlock_init(NAME) 0 # define glthread_rwlock_rdlock(NAME) 0 # define glthread_rwlock_wrlock(NAME) 0 # define glthread_rwlock_unlock(NAME) 0 # define glthread_rwlock_destroy(NAME) 0 /* --------------------- gl_recursive_lock_t datatype --------------------- */ typedef int gl_recursive_lock_t; # define gl_recursive_lock_define(STORAGECLASS, NAME) # define gl_recursive_lock_define_initialized(STORAGECLASS, NAME) # define glthread_recursive_lock_init(NAME) 0 # define glthread_recursive_lock_lock(NAME) 0 # define glthread_recursive_lock_unlock(NAME) 0 # define glthread_recursive_lock_destroy(NAME) 0 /* -------------------------- gl_once_t datatype -------------------------- */ typedef int gl_once_t; # define gl_once_define(STORAGECLASS, NAME) \ STORAGECLASS gl_once_t NAME = 0; # define glthread_once(ONCE_CONTROL, INITFUNCTION) \ (*(ONCE_CONTROL) == 0 ? (*(ONCE_CONTROL) = ~ 0, INITFUNCTION (), 0) : 0) #endif /* ========================================================================= */ /* Macros with built-in error handling. */ /* -------------------------- gl_lock_t datatype -------------------------- */ #define gl_lock_init(NAME) \ do \ { \ if (glthread_lock_init (&NAME)) \ abort (); \ } \ while (0) #define gl_lock_lock(NAME) \ do \ { \ if (glthread_lock_lock (&NAME)) \ abort (); \ } \ while (0) #define gl_lock_unlock(NAME) \ do \ { \ if (glthread_lock_unlock (&NAME)) \ abort (); \ } \ while (0) #define gl_lock_destroy(NAME) \ do \ { \ if (glthread_lock_destroy (&NAME)) \ abort (); \ } \ while (0) /* ------------------------- gl_rwlock_t datatype ------------------------- */ #define gl_rwlock_init(NAME) \ do \ { \ if (glthread_rwlock_init (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_rdlock(NAME) \ do \ { \ if (glthread_rwlock_rdlock (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_wrlock(NAME) \ do \ { \ if (glthread_rwlock_wrlock (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_unlock(NAME) \ do \ { \ if (glthread_rwlock_unlock (&NAME)) \ abort (); \ } \ while (0) #define gl_rwlock_destroy(NAME) \ do \ { \ if (glthread_rwlock_destroy (&NAME)) \ abort (); \ } \ while (0) /* --------------------- gl_recursive_lock_t datatype --------------------- */ #define gl_recursive_lock_init(NAME) \ do \ { \ if (glthread_recursive_lock_init (&NAME)) \ abort (); \ } \ while (0) #define gl_recursive_lock_lock(NAME) \ do \ { \ if (glthread_recursive_lock_lock (&NAME)) \ abort (); \ } \ while (0) #define gl_recursive_lock_unlock(NAME) \ do \ { \ if (glthread_recursive_lock_unlock (&NAME)) \ abort (); \ } \ while (0) #define gl_recursive_lock_destroy(NAME) \ do \ { \ if (glthread_recursive_lock_destroy (&NAME)) \ abort (); \ } \ while (0) /* -------------------------- gl_once_t datatype -------------------------- */ #define gl_once(NAME, INITFUNCTION) \ do \ { \ if (glthread_once (&NAME, INITFUNCTION)) \ abort (); \ } \ while (0) /* ========================================================================= */ #endif /* _LOCK_H */ gnuastro-0.5/bootstrapped/README0000644000175000017500000000251113044627563013540 00000000000000Imported files to GNU Astronomy Utilities ========================================= The contents of this directory (except this README file!) are imported to GNU Astronomy Utilities (Gnuastro) from other projects. Therefore they are not maintained by Gnuastro developers and are kept separately in this directory for clarity and easy maintenance. In the version controlled repository this directory only contains this single README file. It is populated during the bootstrapping process (see ../README-hacking for more on bootstrapping, or the "Bootstrapping" section in the manual). In the distribution tar-ball this directory is populated with the necessary files. The projects that were used are: - GNU Portability Library (Gnulib): https://www.gnu.org/software/gnulib/ This is a very useful collection of libraries (from GNU C library) to enable non-complying operating systems to run programs based on it. It also contains various very useful scripts needed for the GNU build process. - GNU Autoconf-archives: https://www.gnu.org/software/autoconf-archive/ These archives contain a large number of M4 scripts that can be used at ./configure time. We are most grateful to the maintainers of these projects which allow Gnuastro to be easily installed on a very large set of Unix-like operating systems.gnuastro-0.5/bootstrapped/m4/0000755000175000017500000000000013217220465013251 500000000000000gnuastro-0.5/bootstrapped/m4/yield.m40000644000175000017500000000135713217200022014532 00000000000000# yield.m4 serial 2 dnl Copyright (C) 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_YIELD], [ AC_REQUIRE([gl_THREADLIB]) dnl On some systems, sched_yield is in librt, rather than in libpthread. YIELD_LIB= if test $gl_threads_api = posix; then dnl Solaris has sched_yield in librt, not in libpthread or libc. AC_CHECK_LIB([rt], [sched_yield], [YIELD_LIB=-lrt], [dnl Solaris 2.5.1, 2.6 has sched_yield in libposix4, not librt. AC_CHECK_LIB([posix4], [sched_yield], [YIELD_LIB=-lposix4])]) fi AC_SUBST([YIELD_LIB]) ]) gnuastro-0.5/bootstrapped/m4/xsize.m40000644000175000017500000000062613217200022014564 00000000000000# xsize.m4 serial 5 dnl Copyright (C) 2003-2004, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_XSIZE], [ dnl Prerequisites of lib/xsize.h. AC_REQUIRE([gl_SIZE_MAX]) AC_CHECK_HEADERS([stdint.h]) ]) gnuastro-0.5/bootstrapped/m4/wint_t.m40000644000175000017500000000444313217200022014727 00000000000000# wint_t.m4 serial 7 dnl Copyright (C) 2003, 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Test whether has the 'wint_t' type and whether gnulib's dnl or would, if present, override 'wint_t'. dnl Prerequisite: AC_PROG_CC AC_DEFUN([gt_TYPE_WINT_T], [ AC_CACHE_CHECK([for wint_t], [gt_cv_c_wint_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include wint_t foo = (wchar_t)'\0';]], [[]])], [gt_cv_c_wint_t=yes], [gt_cv_c_wint_t=no])]) if test $gt_cv_c_wint_t = yes; then AC_DEFINE([HAVE_WINT_T], [1], [Define if you have the 'wint_t' type.]) dnl Determine whether gnulib's or would, if present, dnl override 'wint_t'. AC_CACHE_CHECK([whether wint_t is too small], [gl_cv_type_wint_t_too_small], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include #endif #include int verify[sizeof (wint_t) < sizeof (int) ? -1 : 1]; ]])], [gl_cv_type_wint_t_too_small=no], [gl_cv_type_wint_t_too_small=yes])]) if test $gl_cv_type_wint_t_too_small = yes; then GNULIB_OVERRIDES_WINT_T=1 else GNULIB_OVERRIDES_WINT_T=0 fi else GNULIB_OVERRIDES_WINT_T=0 fi AC_SUBST([GNULIB_OVERRIDES_WINT_T]) ]) dnl Prerequisites of the 'wint_t' override. AC_DEFUN([gl_TYPE_WINT_T_PREREQ], [ AC_CHECK_HEADERS_ONCE([crtdefs.h]) if test $ac_cv_header_crtdefs_h = yes; then HAVE_CRTDEFS_H=1 else HAVE_CRTDEFS_H=0 fi AC_SUBST([HAVE_CRTDEFS_H]) ]) gnuastro-0.5/bootstrapped/m4/wcwidth.m40000644000175000017500000000665213217200022015100 00000000000000# wcwidth.m4 serial 25 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCWIDTH], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl Persuade glibc to declare wcwidth(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) AC_CHECK_HEADERS_ONCE([wchar.h]) AC_CHECK_FUNCS_ONCE([wcwidth]) AC_CHECK_DECLS([wcwidth], [], [], [[ /* AIX 3.2.5 declares wcwidth in . */ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_wcwidth != yes; then HAVE_DECL_WCWIDTH=0 fi if test $ac_cv_func_wcwidth != yes; then AC_CACHE_CHECK([whether wcwidth is a macro], [gl_cv_func_wcwidth_macro], [AC_EGREP_CPP([wchar_header_defines_wcwidth], [ #include #ifdef wcwidth wchar_header_defines_wcwidth #endif], [gl_cv_func_wcwidth_macro=yes], [gl_cv_func_wcwidth_macro=no]) ]) fi if test $ac_cv_func_wcwidth = yes || test $gl_cv_func_wcwidth_macro = yes; then HAVE_WCWIDTH=1 dnl On Mac OS X 10.3, wcwidth(0x0301) (COMBINING ACUTE ACCENT) returns 1. dnl On OpenBSD 5.0, wcwidth(0x05B0) (HEBREW POINT SHEVA) returns 1. dnl On OSF/1 5.1, wcwidth(0x200B) (ZERO WIDTH SPACE) returns 1. dnl On OpenBSD 5.8, wcwidth(0xFF1A) (FULLWIDTH COLON) returns 0. dnl This leads to bugs in 'ls' (coreutils). AC_CACHE_CHECK([whether wcwidth works reasonably in UTF-8 locales], [gl_cv_func_wcwidth_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include /* AIX 3.2.5 declares wcwidth in . */ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if !HAVE_DECL_WCWIDTH extern # ifdef __cplusplus "C" # endif int wcwidth (int); #endif int main () { int result = 0; if (setlocale (LC_ALL, "fr_FR.UTF-8") != NULL) { if (wcwidth (0x0301) > 0) result |= 1; if (wcwidth (0x05B0) > 0) result |= 2; if (wcwidth (0x200B) > 0) result |= 4; if (wcwidth (0xFF1A) == 0) result |= 8; } return result; }]])], [gl_cv_func_wcwidth_works=yes], [gl_cv_func_wcwidth_works=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc and AIX 7 systems. *-gnu* | aix[7-9]*) gl_cv_func_wcwidth_works="guessing yes";; *) gl_cv_func_wcwidth_works="guessing no";; esac changequote([,])dnl ]) ]) case "$gl_cv_func_wcwidth_works" in *yes) ;; *no) REPLACE_WCWIDTH=1 ;; esac else HAVE_WCWIDTH=0 fi dnl We don't substitute HAVE_WCWIDTH. We assume that if the system does not dnl have the wcwidth function, then it does not declare it. ]) gnuastro-0.5/bootstrapped/m4/wctype_h.m40000644000175000017500000001557513217200022015255 00000000000000# wctype_h.m4 serial 21 dnl A placeholder for ISO C99 , for platforms that lack it. dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. AC_DEFUN([gl_WCTYPE_H], [ AC_REQUIRE([gl_WCTYPE_H_DEFAULTS]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS_ONCE([iswcntrl]) if test $ac_cv_func_iswcntrl = yes; then HAVE_ISWCNTRL=1 else HAVE_ISWCNTRL=0 fi AC_SUBST([HAVE_ISWCNTRL]) AC_REQUIRE([gt_TYPE_WINT_T]) if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi AC_SUBST([HAVE_WINT_T]) AC_REQUIRE([gl_TYPE_WINT_T_PREREQ]) gl_CHECK_NEXT_HEADERS([wctype.h]) if test $ac_cv_header_wctype_h = yes; then if test $ac_cv_func_iswcntrl = yes; then dnl Linux libc5 has an iswprint function that returns 0 for all arguments. dnl The other functions are likely broken in the same way. AC_CACHE_CHECK([whether iswcntrl works], [gl_cv_func_iswcntrl_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { return iswprint ('x') == 0; } ]])], [gl_cv_func_iswcntrl_works=yes], [gl_cv_func_iswcntrl_works=no], [dnl Guess no on Linux libc5, yes otherwise. AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include #if __GNU_LIBRARY__ == 1 Linux libc5 i18n is broken. #endif]], [])], [gl_cv_func_iswcntrl_works="guessing yes"], [gl_cv_func_iswcntrl_works="guessing no"]) ]) ]) fi HAVE_WCTYPE_H=1 else HAVE_WCTYPE_H=0 fi AC_SUBST([HAVE_WCTYPE_H]) case "$gl_cv_func_iswcntrl_works" in *yes) REPLACE_ISWCNTRL=0 ;; *) REPLACE_ISWCNTRL=1 ;; esac AC_SUBST([REPLACE_ISWCNTRL]) if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then dnl Redefine all of iswcntrl, ..., iswxdigit in . : fi if test $REPLACE_ISWCNTRL = 1; then REPLACE_TOWLOWER=1 else AC_CHECK_FUNCS([towlower]) if test $ac_cv_func_towlower = yes; then REPLACE_TOWLOWER=0 else AC_CHECK_DECLS([towlower],,, [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif ]]) if test $ac_cv_have_decl_towlower = yes; then dnl On Minix 3.1.8, the system's declares towlower() and dnl towupper() although it does not have the functions. Avoid a dnl collision with gnulib's replacement. REPLACE_TOWLOWER=1 else REPLACE_TOWLOWER=0 fi fi fi AC_SUBST([REPLACE_TOWLOWER]) if test $HAVE_ISWCNTRL = 0 || test $REPLACE_TOWLOWER = 1; then dnl Redefine towlower, towupper in . : fi dnl We assume that the wctype() and iswctype() functions exist if and only dnl if the type wctype_t is defined in or in if that dnl exists. dnl HP-UX 11.00 declares all these in and lacks . AC_CACHE_CHECK([for wctype_t], [gl_cv_type_wctype_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #if HAVE_WCTYPE_H # include #endif wctype_t a; ]], [[]])], [gl_cv_type_wctype_t=yes], [gl_cv_type_wctype_t=no]) ]) if test $gl_cv_type_wctype_t = no; then HAVE_WCTYPE_T=0 fi dnl We assume that the wctrans() and towctrans() functions exist if and only dnl if the type wctrans_t is defined in . AC_CACHE_CHECK([for wctrans_t], [gl_cv_type_wctrans_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include wctrans_t a; ]], [[]])], [gl_cv_type_wctrans_t=yes], [gl_cv_type_wctrans_t=no]) ]) if test $gl_cv_type_wctrans_t = no; then HAVE_WCTRANS_T=0 fi dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # include #endif #include ]], [wctype iswctype wctrans towctrans ]) ]) AC_DEFUN([gl_WCTYPE_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_WCTYPE_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_WCTYPE_H_DEFAULTS], [ GNULIB_ISWBLANK=0; AC_SUBST([GNULIB_ISWBLANK]) GNULIB_WCTYPE=0; AC_SUBST([GNULIB_WCTYPE]) GNULIB_ISWCTYPE=0; AC_SUBST([GNULIB_ISWCTYPE]) GNULIB_WCTRANS=0; AC_SUBST([GNULIB_WCTRANS]) GNULIB_TOWCTRANS=0; AC_SUBST([GNULIB_TOWCTRANS]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_ISWBLANK=1; AC_SUBST([HAVE_ISWBLANK]) HAVE_WCTYPE_T=1; AC_SUBST([HAVE_WCTYPE_T]) HAVE_WCTRANS_T=1; AC_SUBST([HAVE_WCTRANS_T]) REPLACE_ISWBLANK=0; AC_SUBST([REPLACE_ISWBLANK]) ]) gnuastro-0.5/bootstrapped/m4/wctomb.m40000644000175000017500000000071413217200022014713 00000000000000# wctomb.m4 serial 2 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCTOMB], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) if false; then REPLACE_WCTOMB=1 fi ]) # Prerequisites of lib/wctomb.c. AC_DEFUN([gl_PREREQ_WCTOMB], [ : ]) gnuastro-0.5/bootstrapped/m4/wctob.m40000644000175000017500000000705713217200022014545 00000000000000# wctob.m4 serial 11 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCTOB], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([wctob]) if test $ac_cv_func_wctob = no; then HAVE_WCTOB=0 HAVE_DECL_WCTOB=0 else HAVE_WCTOB=1 dnl Solaris 9 has the wctob() function but it does not work. dnl Cygwin 1.7.2 has the wctob() function but it clobbers caller-owned dnl registers, see . AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether wctob works], [gl_cv_func_wctob_works], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris <= 9 and Cygwin. solaris2.[1-9] | solaris2.[1-9].* | cygwin*) gl_cv_func_wctob_works="guessing no" ;; # Guess no on native Windows. mingw*) gl_cv_func_wctob_works="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_wctob_works="guessing yes" ;; esac changequote([,])dnl case "$host_os" in cygwin*) AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include register long global __asm__ ("%ebx"); int main () { setlocale (LC_ALL, "en_US.UTF-8"); global = 0x12345678; if (wctob (0x00FC) != -1) return 1; if (global != 0x12345678) return 2; return 0; }]])], [:], [gl_cv_func_wctob_works=no], [:]) ;; esac if test "$gl_cv_func_wctob_works" != no && test $LOCALE_FR != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { wchar_t wc; if (mbtowc (&wc, "\374", 1) == 1) if (wctob (wc) != (unsigned char) '\374') return 1; } return 0; }]])], [gl_cv_func_wctob_works=yes], [gl_cv_func_wctob_works=no], [:]) fi ]) case "$gl_cv_func_wctob_works" in *yes) ;; *) REPLACE_WCTOB=1 ;; esac if test $REPLACE_WCTOB = 0; then dnl IRIX 6.5 has the wctob() function but does not declare it. AC_CHECK_DECLS([wctob], [], [], [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_wctob != yes; then HAVE_DECL_WCTOB=0 fi fi fi ]) # Prerequisites of lib/wctob.c. AC_DEFUN([gl_PREREQ_WCTOB], [ : ]) gnuastro-0.5/bootstrapped/m4/wcrtomb.m40000644000175000017500000000703513217200022015100 00000000000000# wcrtomb.m4 serial 12 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_WCRTOMB], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) gl_MBSTATE_T_BROKEN AC_CHECK_FUNCS_ONCE([wcrtomb]) if test $ac_cv_func_wcrtomb = no; then HAVE_WCRTOMB=0 AC_CHECK_DECLS([wcrtomb],,, [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_wcrtomb = yes; then dnl On Minix 3.1.8, the system's declares wcrtomb() although dnl it does not have the function. Avoid a collision with gnulib's dnl replacement. REPLACE_WCRTOMB=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_WCRTOMB=1 else dnl On AIX 4.3, OSF/1 5.1 and Solaris 10, wcrtomb (NULL, 0, NULL) sometimes dnl returns 0 instead of 1. AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([gt_LOCALE_JA]) AC_REQUIRE([gt_LOCALE_ZH_CN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether wcrtomb return value is correct], [gl_cv_func_wcrtomb_retval], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on AIX 4, OSF/1 and Solaris. aix4* | osf* | solaris*) gl_cv_func_wcrtomb_retval="guessing no" ;; # Guess yes on native Windows. mingw*) gl_cv_func_wcrtomb_retval="guessing yes" ;; # Guess yes otherwise. *) gl_cv_func_wcrtomb_retval="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR != none || test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none || test $LOCALE_ZH_CN != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 1; } if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 2; } if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 4; } if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { if (wcrtomb (NULL, 0, NULL) != 1) result |= 8; } return result; }]])], [gl_cv_func_wcrtomb_retval=yes], [gl_cv_func_wcrtomb_retval=no], [:]) fi ]) case "$gl_cv_func_wcrtomb_retval" in *yes) ;; *) REPLACE_WCRTOMB=1 ;; esac fi fi ]) # Prerequisites of lib/wcrtomb.c. AC_DEFUN([gl_PREREQ_WCRTOMB], [ : ]) gnuastro-0.5/bootstrapped/m4/wchar_t.m40000644000175000017500000000146213217200022015050 00000000000000# wchar_t.m4 serial 4 (gettext-0.18.2) dnl Copyright (C) 2002-2003, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Test whether has the 'wchar_t' type. dnl Prerequisite: AC_PROG_CC AC_DEFUN([gt_TYPE_WCHAR_T], [ AC_CACHE_CHECK([for wchar_t], [gt_cv_c_wchar_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include wchar_t foo = (wchar_t)'\0';]], [[]])], [gt_cv_c_wchar_t=yes], [gt_cv_c_wchar_t=no])]) if test $gt_cv_c_wchar_t = yes; then AC_DEFINE([HAVE_WCHAR_T], [1], [Define if you have the 'wchar_t' type.]) fi ]) gnuastro-0.5/bootstrapped/m4/wchar_h.m40000644000175000017500000002354413217200022015041 00000000000000dnl A placeholder for ISO C99 , for platforms that have issues. dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Eric Blake. # wchar_h.m4 serial 42 AC_DEFUN([gl_WCHAR_H], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([gl_WCHAR_H_INLINE_OK]) dnl Prepare for creating substitute . dnl Check for (missing in Linux uClibc when built without wide dnl character support). dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([wchar.h]) if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi AC_SUBST([HAVE_WCHAR_H]) AC_REQUIRE([gl_FEATURES_H]) AC_REQUIRE([gt_TYPE_WINT_T]) if test $gt_cv_c_wint_t = yes; then HAVE_WINT_T=1 else HAVE_WINT_T=0 fi AC_SUBST([HAVE_WINT_T]) AC_REQUIRE([gl_TYPE_WINT_T_PREREQ]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include #endif #include ]], [btowc wctob mbsinit mbrtowc mbrlen mbsrtowcs mbsnrtowcs wcrtomb wcsrtombs wcsnrtombs wcwidth wmemchr wmemcmp wmemcpy wmemmove wmemset wcslen wcsnlen wcscpy wcpcpy wcsncpy wcpncpy wcscat wcsncat wcscmp wcsncmp wcscasecmp wcsncasecmp wcscoll wcsxfrm wcsdup wcschr wcsrchr wcscspn wcsspn wcspbrk wcsstr wcstok wcswidth wcsftime ]) ]) dnl Check whether is usable at all. AC_DEFUN([gl_WCHAR_H_INLINE_OK], [ dnl Test whether suffers due to the transition from '__inline' to dnl 'gnu_inline'. See dnl and . In summary, dnl glibc version 2.5 or older, together with gcc version 4.3 or newer and dnl the option -std=c99 or -std=gnu99, leads to a broken . AC_CACHE_CHECK([whether uses 'inline' correctly], [gl_cv_header_wchar_h_correct_inline], [gl_cv_header_wchar_h_correct_inline=yes AC_LANG_CONFTEST([ AC_LANG_SOURCE([[#define wcstod renamed_wcstod /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include extern int zero (void); int main () { return zero(); } ]])]) dnl Do not rename the object file from conftest.$ac_objext to dnl conftest1.$ac_objext, as this will cause the link to fail on dnl z/OS when using the XPLINK object format (due to duplicate dnl CSECT names). Instead, temporarily redefine $ac_compile so dnl that the object file has the latter name from the start. save_ac_compile="$ac_compile" ac_compile=`echo "$save_ac_compile" | sed s/conftest/conftest1/` if AC_TRY_EVAL([ac_compile]); then AC_LANG_CONFTEST([ AC_LANG_SOURCE([[#define wcstod renamed_wcstod /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int zero (void) { return 0; } ]])]) dnl See note above about renaming object files. ac_compile=`echo "$save_ac_compile" | sed s/conftest/conftest2/` if AC_TRY_EVAL([ac_compile]); then if $CC -o conftest$ac_exeext $CFLAGS $LDFLAGS conftest1.$ac_objext conftest2.$ac_objext $LIBS >&AS_MESSAGE_LOG_FD 2>&1; then : else gl_cv_header_wchar_h_correct_inline=no fi fi fi ac_compile="$save_ac_compile" rm -f conftest1.$ac_objext conftest2.$ac_objext conftest$ac_exeext ]) if test $gl_cv_header_wchar_h_correct_inline = no; then AC_MSG_ERROR([ cannot be used with this compiler ($CC $CFLAGS $CPPFLAGS). This is a known interoperability problem of glibc <= 2.5 with gcc >= 4.3 in C99 mode. You have four options: - Add the flag -fgnu89-inline to CC and reconfigure, or - Fix your include files, using parts of , or - Use a gcc version older than 4.3, or - Don't use the flags -std=c99 or -std=gnu99. Configuration aborted.]) fi ]) AC_DEFUN([gl_WCHAR_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_WCHAR_H_DEFAULTS], [ GNULIB_BTOWC=0; AC_SUBST([GNULIB_BTOWC]) GNULIB_WCTOB=0; AC_SUBST([GNULIB_WCTOB]) GNULIB_MBSINIT=0; AC_SUBST([GNULIB_MBSINIT]) GNULIB_MBRTOWC=0; AC_SUBST([GNULIB_MBRTOWC]) GNULIB_MBRLEN=0; AC_SUBST([GNULIB_MBRLEN]) GNULIB_MBSRTOWCS=0; AC_SUBST([GNULIB_MBSRTOWCS]) GNULIB_MBSNRTOWCS=0; AC_SUBST([GNULIB_MBSNRTOWCS]) GNULIB_WCRTOMB=0; AC_SUBST([GNULIB_WCRTOMB]) GNULIB_WCSRTOMBS=0; AC_SUBST([GNULIB_WCSRTOMBS]) GNULIB_WCSNRTOMBS=0; AC_SUBST([GNULIB_WCSNRTOMBS]) GNULIB_WCWIDTH=0; AC_SUBST([GNULIB_WCWIDTH]) GNULIB_WMEMCHR=0; AC_SUBST([GNULIB_WMEMCHR]) GNULIB_WMEMCMP=0; AC_SUBST([GNULIB_WMEMCMP]) GNULIB_WMEMCPY=0; AC_SUBST([GNULIB_WMEMCPY]) GNULIB_WMEMMOVE=0; AC_SUBST([GNULIB_WMEMMOVE]) GNULIB_WMEMSET=0; AC_SUBST([GNULIB_WMEMSET]) GNULIB_WCSLEN=0; AC_SUBST([GNULIB_WCSLEN]) GNULIB_WCSNLEN=0; AC_SUBST([GNULIB_WCSNLEN]) GNULIB_WCSCPY=0; AC_SUBST([GNULIB_WCSCPY]) GNULIB_WCPCPY=0; AC_SUBST([GNULIB_WCPCPY]) GNULIB_WCSNCPY=0; AC_SUBST([GNULIB_WCSNCPY]) GNULIB_WCPNCPY=0; AC_SUBST([GNULIB_WCPNCPY]) GNULIB_WCSCAT=0; AC_SUBST([GNULIB_WCSCAT]) GNULIB_WCSNCAT=0; AC_SUBST([GNULIB_WCSNCAT]) GNULIB_WCSCMP=0; AC_SUBST([GNULIB_WCSCMP]) GNULIB_WCSNCMP=0; AC_SUBST([GNULIB_WCSNCMP]) GNULIB_WCSCASECMP=0; AC_SUBST([GNULIB_WCSCASECMP]) GNULIB_WCSNCASECMP=0; AC_SUBST([GNULIB_WCSNCASECMP]) GNULIB_WCSCOLL=0; AC_SUBST([GNULIB_WCSCOLL]) GNULIB_WCSXFRM=0; AC_SUBST([GNULIB_WCSXFRM]) GNULIB_WCSDUP=0; AC_SUBST([GNULIB_WCSDUP]) GNULIB_WCSCHR=0; AC_SUBST([GNULIB_WCSCHR]) GNULIB_WCSRCHR=0; AC_SUBST([GNULIB_WCSRCHR]) GNULIB_WCSCSPN=0; AC_SUBST([GNULIB_WCSCSPN]) GNULIB_WCSSPN=0; AC_SUBST([GNULIB_WCSSPN]) GNULIB_WCSPBRK=0; AC_SUBST([GNULIB_WCSPBRK]) GNULIB_WCSSTR=0; AC_SUBST([GNULIB_WCSSTR]) GNULIB_WCSTOK=0; AC_SUBST([GNULIB_WCSTOK]) GNULIB_WCSWIDTH=0; AC_SUBST([GNULIB_WCSWIDTH]) GNULIB_WCSFTIME=0; AC_SUBST([GNULIB_WCSFTIME]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_BTOWC=1; AC_SUBST([HAVE_BTOWC]) HAVE_MBSINIT=1; AC_SUBST([HAVE_MBSINIT]) HAVE_MBRTOWC=1; AC_SUBST([HAVE_MBRTOWC]) HAVE_MBRLEN=1; AC_SUBST([HAVE_MBRLEN]) HAVE_MBSRTOWCS=1; AC_SUBST([HAVE_MBSRTOWCS]) HAVE_MBSNRTOWCS=1; AC_SUBST([HAVE_MBSNRTOWCS]) HAVE_WCRTOMB=1; AC_SUBST([HAVE_WCRTOMB]) HAVE_WCSRTOMBS=1; AC_SUBST([HAVE_WCSRTOMBS]) HAVE_WCSNRTOMBS=1; AC_SUBST([HAVE_WCSNRTOMBS]) HAVE_WMEMCHR=1; AC_SUBST([HAVE_WMEMCHR]) HAVE_WMEMCMP=1; AC_SUBST([HAVE_WMEMCMP]) HAVE_WMEMCPY=1; AC_SUBST([HAVE_WMEMCPY]) HAVE_WMEMMOVE=1; AC_SUBST([HAVE_WMEMMOVE]) HAVE_WMEMSET=1; AC_SUBST([HAVE_WMEMSET]) HAVE_WCSLEN=1; AC_SUBST([HAVE_WCSLEN]) HAVE_WCSNLEN=1; AC_SUBST([HAVE_WCSNLEN]) HAVE_WCSCPY=1; AC_SUBST([HAVE_WCSCPY]) HAVE_WCPCPY=1; AC_SUBST([HAVE_WCPCPY]) HAVE_WCSNCPY=1; AC_SUBST([HAVE_WCSNCPY]) HAVE_WCPNCPY=1; AC_SUBST([HAVE_WCPNCPY]) HAVE_WCSCAT=1; AC_SUBST([HAVE_WCSCAT]) HAVE_WCSNCAT=1; AC_SUBST([HAVE_WCSNCAT]) HAVE_WCSCMP=1; AC_SUBST([HAVE_WCSCMP]) HAVE_WCSNCMP=1; AC_SUBST([HAVE_WCSNCMP]) HAVE_WCSCASECMP=1; AC_SUBST([HAVE_WCSCASECMP]) HAVE_WCSNCASECMP=1; AC_SUBST([HAVE_WCSNCASECMP]) HAVE_WCSCOLL=1; AC_SUBST([HAVE_WCSCOLL]) HAVE_WCSXFRM=1; AC_SUBST([HAVE_WCSXFRM]) HAVE_WCSDUP=1; AC_SUBST([HAVE_WCSDUP]) HAVE_WCSCHR=1; AC_SUBST([HAVE_WCSCHR]) HAVE_WCSRCHR=1; AC_SUBST([HAVE_WCSRCHR]) HAVE_WCSCSPN=1; AC_SUBST([HAVE_WCSCSPN]) HAVE_WCSSPN=1; AC_SUBST([HAVE_WCSSPN]) HAVE_WCSPBRK=1; AC_SUBST([HAVE_WCSPBRK]) HAVE_WCSSTR=1; AC_SUBST([HAVE_WCSSTR]) HAVE_WCSTOK=1; AC_SUBST([HAVE_WCSTOK]) HAVE_WCSWIDTH=1; AC_SUBST([HAVE_WCSWIDTH]) HAVE_WCSFTIME=1; AC_SUBST([HAVE_WCSFTIME]) HAVE_DECL_WCTOB=1; AC_SUBST([HAVE_DECL_WCTOB]) HAVE_DECL_WCWIDTH=1; AC_SUBST([HAVE_DECL_WCWIDTH]) REPLACE_MBSTATE_T=0; AC_SUBST([REPLACE_MBSTATE_T]) REPLACE_BTOWC=0; AC_SUBST([REPLACE_BTOWC]) REPLACE_WCTOB=0; AC_SUBST([REPLACE_WCTOB]) REPLACE_MBSINIT=0; AC_SUBST([REPLACE_MBSINIT]) REPLACE_MBRTOWC=0; AC_SUBST([REPLACE_MBRTOWC]) REPLACE_MBRLEN=0; AC_SUBST([REPLACE_MBRLEN]) REPLACE_MBSRTOWCS=0; AC_SUBST([REPLACE_MBSRTOWCS]) REPLACE_MBSNRTOWCS=0; AC_SUBST([REPLACE_MBSNRTOWCS]) REPLACE_WCRTOMB=0; AC_SUBST([REPLACE_WCRTOMB]) REPLACE_WCSRTOMBS=0; AC_SUBST([REPLACE_WCSRTOMBS]) REPLACE_WCSNRTOMBS=0; AC_SUBST([REPLACE_WCSNRTOMBS]) REPLACE_WCWIDTH=0; AC_SUBST([REPLACE_WCWIDTH]) REPLACE_WCSWIDTH=0; AC_SUBST([REPLACE_WCSWIDTH]) REPLACE_WCSFTIME=0; AC_SUBST([REPLACE_WCSFTIME]) ]) gnuastro-0.5/bootstrapped/m4/warn-on-use.m40000644000175000017500000000415413217200022015575 00000000000000# warn-on-use.m4 serial 5 dnl Copyright (C) 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # gl_WARN_ON_USE_PREPARE(INCLUDES, NAMES) # --------------------------------------- # For each whitespace-separated element in the list of NAMES, define # HAVE_RAW_DECL_name if the function has a declaration among INCLUDES # even after being undefined as a macro. # # See warn-on-use.h for some hints on how to poison function names, as # well as ideas on poisoning global variables and macros. NAMES may # include global variables, but remember that only functions work with # _GL_WARN_ON_USE. Typically, INCLUDES only needs to list a single # header, but if the replacement header pulls in other headers because # some systems declare functions in the wrong header, then INCLUDES # should do likewise. # # It is generally safe to assume declarations for functions declared # in the intersection of C89 and C11 (such as printf) without # needing gl_WARN_ON_USE_PREPARE. AC_DEFUN([gl_WARN_ON_USE_PREPARE], [ m4_foreach_w([gl_decl], [$2], [AH_TEMPLATE([HAVE_RAW_DECL_]AS_TR_CPP(m4_defn([gl_decl])), [Define to 1 if ]m4_defn([gl_decl])[ is declared even after undefining macros.])])dnl dnl FIXME: gl_Symbol must be used unquoted until we can assume dnl autoconf 2.64 or newer. for gl_func in m4_flatten([$2]); do AS_VAR_PUSHDEF([gl_Symbol], [gl_cv_have_raw_decl_$gl_func])dnl AC_CACHE_CHECK([whether $gl_func is declared without a macro], gl_Symbol, [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([$1], [@%:@undef $gl_func (void) $gl_func;])], [AS_VAR_SET(gl_Symbol, [yes])], [AS_VAR_SET(gl_Symbol, [no])])]) AS_VAR_IF(gl_Symbol, [yes], [AC_DEFINE_UNQUOTED(AS_TR_CPP([HAVE_RAW_DECL_$gl_func]), [1]) dnl shortcut - if the raw declaration exists, then set a cache dnl variable to allow skipping any later AC_CHECK_DECL efforts eval ac_cv_have_decl_$gl_func=yes]) AS_VAR_POPDEF([gl_Symbol])dnl done ]) gnuastro-0.5/bootstrapped/m4/vsnprintf.m40000644000175000017500000000362113217200022015451 00000000000000# vsnprintf.m4 serial 7 dnl Copyright (C) 2002-2004, 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Libintl 0.17 will replace vsnprintf only if it does not support %1$s, dnl but defers to any gnulib vsnprintf replacements. Therefore, gnulib dnl must guarantee that the decision for replacing vsnprintf is a superset dnl of the reasons checked by libintl. AC_DEFUN([gl_FUNC_VSNPRINTF], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) gl_cv_func_vsnprintf_usable=no AC_CHECK_FUNCS([vsnprintf]) if test $ac_cv_func_vsnprintf = yes; then gl_SNPRINTF_SIZE1 case "$gl_cv_func_snprintf_size1" in *yes) gl_SNPRINTF_RETVAL_C99 case "$gl_cv_func_snprintf_retval_c99" in *yes) gl_PRINTF_POSITIONS case "$gl_cv_func_printf_positions" in *yes) gl_cv_func_vsnprintf_usable=yes ;; esac ;; esac ;; esac fi if test $gl_cv_func_vsnprintf_usable = no; then gl_REPLACE_VSNPRINTF fi AC_CHECK_DECLS_ONCE([vsnprintf]) if test $ac_cv_have_decl_vsnprintf = no; then HAVE_DECL_VSNPRINTF=0 fi ]) AC_DEFUN([gl_REPLACE_VSNPRINTF], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) AC_LIBOBJ([vsnprintf]) if test $ac_cv_func_vsnprintf = yes; then REPLACE_VSNPRINTF=1 else AC_CHECK_DECLS_ONCE([vsnprintf]) if test $ac_cv_have_decl_vsnprintf = yes; then dnl If the function is declared but does not appear to exist, it may be dnl defined as an inline function. In order to avoid a conflict, we have dnl to define rpl_vsnprintf, not vsnprintf. REPLACE_VSNPRINTF=1 fi fi gl_PREREQ_VSNPRINTF ]) # Prerequisites of lib/vsnprintf.c. AC_DEFUN([gl_PREREQ_VSNPRINTF], [:]) gnuastro-0.5/bootstrapped/m4/vasnprintf.m40000644000175000017500000002113313217200022015610 00000000000000# vasnprintf.m4 serial 36 dnl Copyright (C) 2002-2004, 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_VASNPRINTF], [ AC_CHECK_FUNCS_ONCE([vasnprintf]) if test $ac_cv_func_vasnprintf = no; then gl_REPLACE_VASNPRINTF fi ]) AC_DEFUN([gl_REPLACE_VASNPRINTF], [ AC_CHECK_FUNCS_ONCE([vasnprintf]) AC_LIBOBJ([vasnprintf]) AC_LIBOBJ([printf-args]) AC_LIBOBJ([printf-parse]) AC_LIBOBJ([asnprintf]) if test $ac_cv_func_vasnprintf = yes; then AC_DEFINE([REPLACE_VASNPRINTF], [1], [Define if vasnprintf exists but is overridden by gnulib.]) fi gl_PREREQ_PRINTF_ARGS gl_PREREQ_PRINTF_PARSE gl_PREREQ_VASNPRINTF gl_PREREQ_ASNPRINTF ]) # Prerequisites of lib/printf-args.h, lib/printf-args.c. AC_DEFUN([gl_PREREQ_PRINTF_ARGS], [ AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) ]) # Prerequisites of lib/printf-parse.h, lib/printf-parse.c. AC_DEFUN([gl_PREREQ_PRINTF_PARSE], [ AC_REQUIRE([gl_FEATURES_H]) AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) AC_REQUIRE([AC_TYPE_SIZE_T]) AC_CHECK_TYPE([ptrdiff_t], , [AC_DEFINE([ptrdiff_t], [long], [Define as the type of the result of subtracting two pointers, if the system doesn't define it.]) ]) AC_REQUIRE([gt_AC_TYPE_INTMAX_T]) ]) # Prerequisites of lib/vasnprintf.c. AC_DEFUN_ONCE([gl_PREREQ_VASNPRINTF], [ AC_REQUIRE([AC_FUNC_ALLOCA]) AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) AC_CHECK_FUNCS([snprintf strnlen wcslen wcsnlen mbrtowc wcrtomb]) dnl Use the _snprintf function only if it is declared (because on NetBSD it dnl is defined as a weak alias of snprintf; we prefer to use the latter). AC_CHECK_DECLS([_snprintf], , , [[#include ]]) dnl Knowing DBL_EXPBIT0_WORD and DBL_EXPBIT0_BIT enables an optimization dnl in the code for NEED_PRINTF_LONG_DOUBLE || NEED_PRINTF_DOUBLE. AC_REQUIRE([gl_DOUBLE_EXPONENT_LOCATION]) dnl We can avoid a lot of code by assuming that snprintf's return value dnl conforms to ISO C99. So check that. AC_REQUIRE([gl_SNPRINTF_RETVAL_C99]) case "$gl_cv_func_snprintf_retval_c99" in *yes) AC_DEFINE([HAVE_SNPRINTF_RETVAL_C99], [1], [Define if the return value of the snprintf function is the number of of bytes (excluding the terminating NUL) that would have been produced if the buffer had been large enough.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting 'long double' # arguments. AC_DEFUN_ONCE([gl_PREREQ_VASNPRINTF_LONG_DOUBLE], [ AC_REQUIRE([gl_PRINTF_LONG_DOUBLE]) case "$gl_cv_func_printf_long_double" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'long double' arguments.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting infinite 'double' # arguments. AC_DEFUN([gl_PREREQ_VASNPRINTF_INFINITE_DOUBLE], [ AC_REQUIRE([gl_PRINTF_INFINITE]) case "$gl_cv_func_printf_infinite" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_INFINITE_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for infinite 'double' arguments.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting infinite 'long double' # arguments. AC_DEFUN([gl_PREREQ_VASNPRINTF_INFINITE_LONG_DOUBLE], [ AC_REQUIRE([gl_PRINTF_INFINITE_LONG_DOUBLE]) dnl There is no need to set NEED_PRINTF_INFINITE_LONG_DOUBLE if dnl NEED_PRINTF_LONG_DOUBLE is already set. AC_REQUIRE([gl_PREREQ_VASNPRINTF_LONG_DOUBLE]) case "$gl_cv_func_printf_long_double" in *yes) case "$gl_cv_func_printf_infinite_long_double" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_INFINITE_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for infinite 'long double' arguments.]) ;; esac ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 'a' directive. AC_DEFUN([gl_PREREQ_VASNPRINTF_DIRECTIVE_A], [ AC_REQUIRE([gl_PRINTF_DIRECTIVE_A]) case "$gl_cv_func_printf_directive_a" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_DIRECTIVE_A], [1], [Define if the vasnprintf implementation needs special code for the 'a' and 'A' directives.]) AC_CHECK_FUNCS([nl_langinfo]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 'F' directive. AC_DEFUN([gl_PREREQ_VASNPRINTF_DIRECTIVE_F], [ AC_REQUIRE([gl_PRINTF_DIRECTIVE_F]) case "$gl_cv_func_printf_directive_f" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_DIRECTIVE_F], [1], [Define if the vasnprintf implementation needs special code for the 'F' directive.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 'ls' directive. AC_DEFUN([gl_PREREQ_VASNPRINTF_DIRECTIVE_LS], [ AC_REQUIRE([gl_PRINTF_DIRECTIVE_LS]) case "$gl_cv_func_printf_directive_ls" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_DIRECTIVE_LS], [1], [Define if the vasnprintf implementation needs special code for the 'ls' directive.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the ' flag. AC_DEFUN([gl_PREREQ_VASNPRINTF_FLAG_GROUPING], [ AC_REQUIRE([gl_PRINTF_FLAG_GROUPING]) case "$gl_cv_func_printf_flag_grouping" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_FLAG_GROUPING], [1], [Define if the vasnprintf implementation needs special code for the ' flag.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the '-' flag. AC_DEFUN([gl_PREREQ_VASNPRINTF_FLAG_LEFTADJUST], [ AC_REQUIRE([gl_PRINTF_FLAG_LEFTADJUST]) case "$gl_cv_func_printf_flag_leftadjust" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_FLAG_LEFTADJUST], [1], [Define if the vasnprintf implementation needs special code for the '-' flag.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting the 0 flag. AC_DEFUN([gl_PREREQ_VASNPRINTF_FLAG_ZERO], [ AC_REQUIRE([gl_PRINTF_FLAG_ZERO]) case "$gl_cv_func_printf_flag_zero" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_FLAG_ZERO], [1], [Define if the vasnprintf implementation needs special code for the 0 flag.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for supporting large precisions. AC_DEFUN([gl_PREREQ_VASNPRINTF_PRECISION], [ AC_REQUIRE([gl_PRINTF_PRECISION]) case "$gl_cv_func_printf_precision" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_UNBOUNDED_PRECISION], [1], [Define if the vasnprintf implementation needs special code for supporting large precisions without arbitrary bounds.]) AC_DEFINE([NEED_PRINTF_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'double' arguments.]) AC_DEFINE([NEED_PRINTF_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'long double' arguments.]) ;; esac ]) # Extra prerequisites of lib/vasnprintf.c for surviving out-of-memory # conditions. AC_DEFUN([gl_PREREQ_VASNPRINTF_ENOMEM], [ AC_REQUIRE([gl_PRINTF_ENOMEM]) case "$gl_cv_func_printf_enomem" in *yes) ;; *) AC_DEFINE([NEED_PRINTF_ENOMEM], [1], [Define if the vasnprintf implementation needs special code for surviving out-of-memory conditions.]) AC_DEFINE([NEED_PRINTF_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'double' arguments.]) AC_DEFINE([NEED_PRINTF_LONG_DOUBLE], [1], [Define if the vasnprintf implementation needs special code for 'long double' arguments.]) ;; esac ]) # Prerequisites of lib/vasnprintf.c including all extras for POSIX compliance. AC_DEFUN([gl_PREREQ_VASNPRINTF_WITH_EXTRAS], [ AC_REQUIRE([gl_PREREQ_VASNPRINTF]) gl_PREREQ_VASNPRINTF_LONG_DOUBLE gl_PREREQ_VASNPRINTF_INFINITE_DOUBLE gl_PREREQ_VASNPRINTF_INFINITE_LONG_DOUBLE gl_PREREQ_VASNPRINTF_DIRECTIVE_A gl_PREREQ_VASNPRINTF_DIRECTIVE_F gl_PREREQ_VASNPRINTF_DIRECTIVE_LS gl_PREREQ_VASNPRINTF_FLAG_GROUPING gl_PREREQ_VASNPRINTF_FLAG_LEFTADJUST gl_PREREQ_VASNPRINTF_FLAG_ZERO gl_PREREQ_VASNPRINTF_PRECISION gl_PREREQ_VASNPRINTF_ENOMEM ]) # Prerequisites of lib/asnprintf.c. AC_DEFUN([gl_PREREQ_ASNPRINTF], [ ]) gnuastro-0.5/bootstrapped/m4/usleep.m40000644000175000017500000000346113217200022014717 00000000000000# usleep.m4 serial 4 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl This macro intentionally does not check for select or nanosleep; dnl both of those modules can require external libraries. AC_DEFUN([gl_FUNC_USLEEP], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) dnl usleep was required in POSIX 2001, but dropped as obsolete in dnl POSIX 2008; therefore, it is not always exposed in headers. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_FUNCS_ONCE([usleep]) AC_CHECK_TYPE([useconds_t], [], [AC_DEFINE([useconds_t], [unsigned int], [Define to an unsigned 32-bit type if lacks this type.])]) if test $ac_cv_func_usleep = no; then HAVE_USLEEP=0 else dnl POSIX allows implementations to reject arguments larger than dnl 999999, but GNU guarantees it will work. AC_CACHE_CHECK([whether usleep allows large arguments], [gl_cv_func_usleep_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include ]], [[return !!usleep (1000000);]])], [gl_cv_func_usleep_works=yes], [gl_cv_func_usleep_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_usleep_works="guessing yes" ;; # Guess no on native Windows. mingw*) gl_cv_func_usleep_works="guessing no" ;; # If we don't know, assume the worst. *) gl_cv_func_usleep_works="guessing no" ;; esac ])]) case "$gl_cv_func_usleep_works" in *yes) ;; *) REPLACE_USLEEP=1 ;; esac fi ]) gnuastro-0.5/bootstrapped/m4/unistd_h.m40000644000175000017500000002235413217200022015241 00000000000000# unistd_h.m4 serial 71 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Simon Josefsson, Bruno Haible. AC_DEFUN([gl_UNISTD_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([unistd.h]) if test $ac_cv_header_unistd_h = yes; then HAVE_UNISTD_H=1 else HAVE_UNISTD_H=0 fi AC_SUBST([HAVE_UNISTD_H]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) dnl Determine WINDOWS_64_BIT_OFF_T. AC_REQUIRE([gl_TYPE_OFF_T]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ #if HAVE_UNISTD_H # include #endif /* Some systems declare various items in the wrong headers. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include # include # include # if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # include # endif #endif ]], [chdir chown dup dup2 dup3 environ euidaccess faccessat fchdir fchownat fdatasync fsync ftruncate getcwd getdomainname getdtablesize getgroups gethostname getlogin getlogin_r getpagesize getusershell setusershell endusershell group_member isatty lchown link linkat lseek pipe pipe2 pread pwrite readlink readlinkat rmdir sethostname sleep symlink symlinkat truncate ttyname_r unlink unlinkat usleep]) ]) AC_DEFUN([gl_UNISTD_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_UNISTD_H_DEFAULTS], [ GNULIB_CHDIR=0; AC_SUBST([GNULIB_CHDIR]) GNULIB_CHOWN=0; AC_SUBST([GNULIB_CHOWN]) GNULIB_CLOSE=0; AC_SUBST([GNULIB_CLOSE]) GNULIB_DUP=0; AC_SUBST([GNULIB_DUP]) GNULIB_DUP2=0; AC_SUBST([GNULIB_DUP2]) GNULIB_DUP3=0; AC_SUBST([GNULIB_DUP3]) GNULIB_ENVIRON=0; AC_SUBST([GNULIB_ENVIRON]) GNULIB_EUIDACCESS=0; AC_SUBST([GNULIB_EUIDACCESS]) GNULIB_FACCESSAT=0; AC_SUBST([GNULIB_FACCESSAT]) GNULIB_FCHDIR=0; AC_SUBST([GNULIB_FCHDIR]) GNULIB_FCHOWNAT=0; AC_SUBST([GNULIB_FCHOWNAT]) GNULIB_FDATASYNC=0; AC_SUBST([GNULIB_FDATASYNC]) GNULIB_FSYNC=0; AC_SUBST([GNULIB_FSYNC]) GNULIB_FTRUNCATE=0; AC_SUBST([GNULIB_FTRUNCATE]) GNULIB_GETCWD=0; AC_SUBST([GNULIB_GETCWD]) GNULIB_GETDOMAINNAME=0; AC_SUBST([GNULIB_GETDOMAINNAME]) GNULIB_GETDTABLESIZE=0; AC_SUBST([GNULIB_GETDTABLESIZE]) GNULIB_GETGROUPS=0; AC_SUBST([GNULIB_GETGROUPS]) GNULIB_GETHOSTNAME=0; AC_SUBST([GNULIB_GETHOSTNAME]) GNULIB_GETLOGIN=0; AC_SUBST([GNULIB_GETLOGIN]) GNULIB_GETLOGIN_R=0; AC_SUBST([GNULIB_GETLOGIN_R]) GNULIB_GETPAGESIZE=0; AC_SUBST([GNULIB_GETPAGESIZE]) GNULIB_GETUSERSHELL=0; AC_SUBST([GNULIB_GETUSERSHELL]) GNULIB_GROUP_MEMBER=0; AC_SUBST([GNULIB_GROUP_MEMBER]) GNULIB_ISATTY=0; AC_SUBST([GNULIB_ISATTY]) GNULIB_LCHOWN=0; AC_SUBST([GNULIB_LCHOWN]) GNULIB_LINK=0; AC_SUBST([GNULIB_LINK]) GNULIB_LINKAT=0; AC_SUBST([GNULIB_LINKAT]) GNULIB_LSEEK=0; AC_SUBST([GNULIB_LSEEK]) GNULIB_PIPE=0; AC_SUBST([GNULIB_PIPE]) GNULIB_PIPE2=0; AC_SUBST([GNULIB_PIPE2]) GNULIB_PREAD=0; AC_SUBST([GNULIB_PREAD]) GNULIB_PWRITE=0; AC_SUBST([GNULIB_PWRITE]) GNULIB_READ=0; AC_SUBST([GNULIB_READ]) GNULIB_READLINK=0; AC_SUBST([GNULIB_READLINK]) GNULIB_READLINKAT=0; AC_SUBST([GNULIB_READLINKAT]) GNULIB_RMDIR=0; AC_SUBST([GNULIB_RMDIR]) GNULIB_SETHOSTNAME=0; AC_SUBST([GNULIB_SETHOSTNAME]) GNULIB_SLEEP=0; AC_SUBST([GNULIB_SLEEP]) GNULIB_SYMLINK=0; AC_SUBST([GNULIB_SYMLINK]) GNULIB_SYMLINKAT=0; AC_SUBST([GNULIB_SYMLINKAT]) GNULIB_TRUNCATE=0; AC_SUBST([GNULIB_TRUNCATE]) GNULIB_TTYNAME_R=0; AC_SUBST([GNULIB_TTYNAME_R]) GNULIB_UNISTD_H_NONBLOCKING=0; AC_SUBST([GNULIB_UNISTD_H_NONBLOCKING]) GNULIB_UNISTD_H_SIGPIPE=0; AC_SUBST([GNULIB_UNISTD_H_SIGPIPE]) GNULIB_UNLINK=0; AC_SUBST([GNULIB_UNLINK]) GNULIB_UNLINKAT=0; AC_SUBST([GNULIB_UNLINKAT]) GNULIB_USLEEP=0; AC_SUBST([GNULIB_USLEEP]) GNULIB_WRITE=0; AC_SUBST([GNULIB_WRITE]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_CHOWN=1; AC_SUBST([HAVE_CHOWN]) HAVE_DUP2=1; AC_SUBST([HAVE_DUP2]) HAVE_DUP3=1; AC_SUBST([HAVE_DUP3]) HAVE_EUIDACCESS=1; AC_SUBST([HAVE_EUIDACCESS]) HAVE_FACCESSAT=1; AC_SUBST([HAVE_FACCESSAT]) HAVE_FCHDIR=1; AC_SUBST([HAVE_FCHDIR]) HAVE_FCHOWNAT=1; AC_SUBST([HAVE_FCHOWNAT]) HAVE_FDATASYNC=1; AC_SUBST([HAVE_FDATASYNC]) HAVE_FSYNC=1; AC_SUBST([HAVE_FSYNC]) HAVE_FTRUNCATE=1; AC_SUBST([HAVE_FTRUNCATE]) HAVE_GETDTABLESIZE=1; AC_SUBST([HAVE_GETDTABLESIZE]) HAVE_GETGROUPS=1; AC_SUBST([HAVE_GETGROUPS]) HAVE_GETHOSTNAME=1; AC_SUBST([HAVE_GETHOSTNAME]) HAVE_GETLOGIN=1; AC_SUBST([HAVE_GETLOGIN]) HAVE_GETPAGESIZE=1; AC_SUBST([HAVE_GETPAGESIZE]) HAVE_GROUP_MEMBER=1; AC_SUBST([HAVE_GROUP_MEMBER]) HAVE_LCHOWN=1; AC_SUBST([HAVE_LCHOWN]) HAVE_LINK=1; AC_SUBST([HAVE_LINK]) HAVE_LINKAT=1; AC_SUBST([HAVE_LINKAT]) HAVE_PIPE=1; AC_SUBST([HAVE_PIPE]) HAVE_PIPE2=1; AC_SUBST([HAVE_PIPE2]) HAVE_PREAD=1; AC_SUBST([HAVE_PREAD]) HAVE_PWRITE=1; AC_SUBST([HAVE_PWRITE]) HAVE_READLINK=1; AC_SUBST([HAVE_READLINK]) HAVE_READLINKAT=1; AC_SUBST([HAVE_READLINKAT]) HAVE_SETHOSTNAME=1; AC_SUBST([HAVE_SETHOSTNAME]) HAVE_SLEEP=1; AC_SUBST([HAVE_SLEEP]) HAVE_SYMLINK=1; AC_SUBST([HAVE_SYMLINK]) HAVE_SYMLINKAT=1; AC_SUBST([HAVE_SYMLINKAT]) HAVE_TRUNCATE=1; AC_SUBST([HAVE_TRUNCATE]) HAVE_UNLINKAT=1; AC_SUBST([HAVE_UNLINKAT]) HAVE_USLEEP=1; AC_SUBST([HAVE_USLEEP]) HAVE_DECL_ENVIRON=1; AC_SUBST([HAVE_DECL_ENVIRON]) HAVE_DECL_FCHDIR=1; AC_SUBST([HAVE_DECL_FCHDIR]) HAVE_DECL_FDATASYNC=1; AC_SUBST([HAVE_DECL_FDATASYNC]) HAVE_DECL_GETDOMAINNAME=1; AC_SUBST([HAVE_DECL_GETDOMAINNAME]) HAVE_DECL_GETLOGIN=1; AC_SUBST([HAVE_DECL_GETLOGIN]) HAVE_DECL_GETLOGIN_R=1; AC_SUBST([HAVE_DECL_GETLOGIN_R]) HAVE_DECL_GETPAGESIZE=1; AC_SUBST([HAVE_DECL_GETPAGESIZE]) HAVE_DECL_GETUSERSHELL=1; AC_SUBST([HAVE_DECL_GETUSERSHELL]) HAVE_DECL_SETHOSTNAME=1; AC_SUBST([HAVE_DECL_SETHOSTNAME]) HAVE_DECL_TTYNAME_R=1; AC_SUBST([HAVE_DECL_TTYNAME_R]) HAVE_OS_H=0; AC_SUBST([HAVE_OS_H]) HAVE_SYS_PARAM_H=0; AC_SUBST([HAVE_SYS_PARAM_H]) REPLACE_CHOWN=0; AC_SUBST([REPLACE_CHOWN]) REPLACE_CLOSE=0; AC_SUBST([REPLACE_CLOSE]) REPLACE_DUP=0; AC_SUBST([REPLACE_DUP]) REPLACE_DUP2=0; AC_SUBST([REPLACE_DUP2]) REPLACE_FACCESSAT=0; AC_SUBST([REPLACE_FACCESSAT]) REPLACE_FCHOWNAT=0; AC_SUBST([REPLACE_FCHOWNAT]) REPLACE_FTRUNCATE=0; AC_SUBST([REPLACE_FTRUNCATE]) REPLACE_GETCWD=0; AC_SUBST([REPLACE_GETCWD]) REPLACE_GETDOMAINNAME=0; AC_SUBST([REPLACE_GETDOMAINNAME]) REPLACE_GETDTABLESIZE=0; AC_SUBST([REPLACE_GETDTABLESIZE]) REPLACE_GETLOGIN_R=0; AC_SUBST([REPLACE_GETLOGIN_R]) REPLACE_GETGROUPS=0; AC_SUBST([REPLACE_GETGROUPS]) REPLACE_GETPAGESIZE=0; AC_SUBST([REPLACE_GETPAGESIZE]) REPLACE_ISATTY=0; AC_SUBST([REPLACE_ISATTY]) REPLACE_LCHOWN=0; AC_SUBST([REPLACE_LCHOWN]) REPLACE_LINK=0; AC_SUBST([REPLACE_LINK]) REPLACE_LINKAT=0; AC_SUBST([REPLACE_LINKAT]) REPLACE_LSEEK=0; AC_SUBST([REPLACE_LSEEK]) REPLACE_PREAD=0; AC_SUBST([REPLACE_PREAD]) REPLACE_PWRITE=0; AC_SUBST([REPLACE_PWRITE]) REPLACE_READ=0; AC_SUBST([REPLACE_READ]) REPLACE_READLINK=0; AC_SUBST([REPLACE_READLINK]) REPLACE_READLINKAT=0; AC_SUBST([REPLACE_READLINKAT]) REPLACE_RMDIR=0; AC_SUBST([REPLACE_RMDIR]) REPLACE_SLEEP=0; AC_SUBST([REPLACE_SLEEP]) REPLACE_SYMLINK=0; AC_SUBST([REPLACE_SYMLINK]) REPLACE_SYMLINKAT=0; AC_SUBST([REPLACE_SYMLINKAT]) REPLACE_TRUNCATE=0; AC_SUBST([REPLACE_TRUNCATE]) REPLACE_TTYNAME_R=0; AC_SUBST([REPLACE_TTYNAME_R]) REPLACE_UNLINK=0; AC_SUBST([REPLACE_UNLINK]) REPLACE_UNLINKAT=0; AC_SUBST([REPLACE_UNLINKAT]) REPLACE_USLEEP=0; AC_SUBST([REPLACE_USLEEP]) REPLACE_WRITE=0; AC_SUBST([REPLACE_WRITE]) UNISTD_H_HAVE_WINSOCK2_H=0; AC_SUBST([UNISTD_H_HAVE_WINSOCK2_H]) UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=0; AC_SUBST([UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS]) ]) gnuastro-0.5/bootstrapped/m4/time_h.m40000644000175000017500000001376213217200022014674 00000000000000# Configure a more-standard replacement for . # Copyright (C) 2000-2001, 2003-2007, 2009-2017 Free Software Foundation, Inc. # serial 11 # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert and Jim Meyering. AC_DEFUN([gl_HEADER_TIME_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_HEADER_TIME_H_BODY]) ]) AC_DEFUN([gl_HEADER_TIME_H_BODY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_TIME_H_DEFAULTS]) gl_NEXT_HEADERS([time.h]) AC_REQUIRE([gl_CHECK_TYPE_STRUCT_TIMESPEC]) ]) dnl Check whether 'struct timespec' is declared dnl in time.h, sys/time.h, pthread.h, or unistd.h. AC_DEFUN([gl_CHECK_TYPE_STRUCT_TIMESPEC], [ AC_CHECK_HEADERS_ONCE([sys/time.h]) AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_time_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_time_h=yes], [gl_cv_sys_struct_timespec_in_time_h=no])]) TIME_H_DEFINES_STRUCT_TIMESPEC=0 SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=0 PTHREAD_H_DEFINES_STRUCT_TIMESPEC=0 UNISTD_H_DEFINES_STRUCT_TIMESPEC=0 if test $gl_cv_sys_struct_timespec_in_time_h = yes; then TIME_H_DEFINES_STRUCT_TIMESPEC=1 else AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_sys_time_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_sys_time_h=yes], [gl_cv_sys_struct_timespec_in_sys_time_h=no])]) if test $gl_cv_sys_struct_timespec_in_sys_time_h = yes; then SYS_TIME_H_DEFINES_STRUCT_TIMESPEC=1 else AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_pthread_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_pthread_h=yes], [gl_cv_sys_struct_timespec_in_pthread_h=no])]) if test $gl_cv_sys_struct_timespec_in_pthread_h = yes; then PTHREAD_H_DEFINES_STRUCT_TIMESPEC=1 else AC_CACHE_CHECK([for struct timespec in ], [gl_cv_sys_struct_timespec_in_unistd_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[static struct timespec x; x.tv_sec = x.tv_nsec;]])], [gl_cv_sys_struct_timespec_in_unistd_h=yes], [gl_cv_sys_struct_timespec_in_unistd_h=no])]) if test $gl_cv_sys_struct_timespec_in_unistd_h = yes; then UNISTD_H_DEFINES_STRUCT_TIMESPEC=1 fi fi fi fi AC_SUBST([TIME_H_DEFINES_STRUCT_TIMESPEC]) AC_SUBST([SYS_TIME_H_DEFINES_STRUCT_TIMESPEC]) AC_SUBST([PTHREAD_H_DEFINES_STRUCT_TIMESPEC]) AC_SUBST([UNISTD_H_DEFINES_STRUCT_TIMESPEC]) ]) AC_DEFUN([gl_TIME_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_TIME_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_HEADER_TIME_H_DEFAULTS], [ GNULIB_CTIME=0; AC_SUBST([GNULIB_CTIME]) GNULIB_MKTIME=0; AC_SUBST([GNULIB_MKTIME]) GNULIB_LOCALTIME=0; AC_SUBST([GNULIB_LOCALTIME]) GNULIB_NANOSLEEP=0; AC_SUBST([GNULIB_NANOSLEEP]) GNULIB_STRFTIME=0; AC_SUBST([GNULIB_STRFTIME]) GNULIB_STRPTIME=0; AC_SUBST([GNULIB_STRPTIME]) GNULIB_TIMEGM=0; AC_SUBST([GNULIB_TIMEGM]) GNULIB_TIME_R=0; AC_SUBST([GNULIB_TIME_R]) GNULIB_TIME_RZ=0; AC_SUBST([GNULIB_TIME_RZ]) GNULIB_TZSET=0; AC_SUBST([GNULIB_TZSET]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_LOCALTIME_R=1; AC_SUBST([HAVE_DECL_LOCALTIME_R]) HAVE_NANOSLEEP=1; AC_SUBST([HAVE_NANOSLEEP]) HAVE_STRPTIME=1; AC_SUBST([HAVE_STRPTIME]) HAVE_TIMEGM=1; AC_SUBST([HAVE_TIMEGM]) HAVE_TZSET=1; AC_SUBST([HAVE_TZSET]) dnl Even GNU libc does not have timezone_t yet. HAVE_TIMEZONE_T=0; AC_SUBST([HAVE_TIMEZONE_T]) dnl If another module says to replace or to not replace, do that. dnl Otherwise, replace only if someone compiles with -DGNULIB_PORTCHECK; dnl this lets maintainers check for portability. REPLACE_CTIME=GNULIB_PORTCHECK; AC_SUBST([REPLACE_CTIME]) REPLACE_LOCALTIME_R=GNULIB_PORTCHECK; AC_SUBST([REPLACE_LOCALTIME_R]) REPLACE_MKTIME=GNULIB_PORTCHECK; AC_SUBST([REPLACE_MKTIME]) REPLACE_NANOSLEEP=GNULIB_PORTCHECK; AC_SUBST([REPLACE_NANOSLEEP]) REPLACE_STRFTIME=GNULIB_PORTCHECK; AC_SUBST([REPLACE_STRFTIME]) REPLACE_TIMEGM=GNULIB_PORTCHECK; AC_SUBST([REPLACE_TIMEGM]) REPLACE_TZSET=GNULIB_PORTCHECK; AC_SUBST([REPLACE_TZSET]) dnl Hack so that the time module doesn't depend on the sys_time module. dnl First, default GNULIB_GETTIMEOFDAY to 0 if sys_time is absent. : ${GNULIB_GETTIMEOFDAY=0}; AC_SUBST([GNULIB_GETTIMEOFDAY]) dnl Second, it's OK to not use GNULIB_PORTCHECK for REPLACE_GMTIME dnl and REPLACE_LOCALTIME, as portability to Solaris 2.6 and earlier dnl is no longer a big deal. REPLACE_GMTIME=0; AC_SUBST([REPLACE_GMTIME]) REPLACE_LOCALTIME=0; AC_SUBST([REPLACE_LOCALTIME]) ]) gnuastro-0.5/bootstrapped/m4/threadlib.m40000644000175000017500000003614213217200022015362 00000000000000# threadlib.m4 serial 13 dnl Copyright (C) 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl gl_THREADLIB dnl ------------ dnl Tests for a multithreading library to be used. dnl If the configure.ac contains a definition of the gl_THREADLIB_DEFAULT_NO dnl (it must be placed before the invocation of gl_THREADLIB_EARLY!), then the dnl default is 'no', otherwise it is system dependent. In both cases, the user dnl can change the choice through the options --enable-threads=choice or dnl --disable-threads. dnl Defines at most one of the macros USE_POSIX_THREADS, USE_SOLARIS_THREADS, dnl USE_PTH_THREADS, USE_WINDOWS_THREADS dnl Sets the variables LIBTHREAD and LTLIBTHREAD to the linker options for use dnl in a Makefile (LIBTHREAD for use without libtool, LTLIBTHREAD for use with dnl libtool). dnl Sets the variables LIBMULTITHREAD and LTLIBMULTITHREAD similarly, for dnl programs that really need multithread functionality. The difference dnl between LIBTHREAD and LIBMULTITHREAD is that on platforms supporting weak dnl symbols, typically LIBTHREAD is empty whereas LIBMULTITHREAD is not. dnl Adds to CPPFLAGS the flag -D_REENTRANT or -D_THREAD_SAFE if needed for dnl multithread-safe programs. AC_DEFUN([gl_THREADLIB_EARLY], [ AC_REQUIRE([gl_THREADLIB_EARLY_BODY]) ]) dnl The guts of gl_THREADLIB_EARLY. Needs to be expanded only once. AC_DEFUN([gl_THREADLIB_EARLY_BODY], [ dnl Ordering constraints: This macro modifies CPPFLAGS in a way that dnl influences the result of the autoconf tests that test for *_unlocked dnl declarations, on AIX 5 at least. Therefore it must come early. AC_BEFORE([$0], [gl_FUNC_GLIBC_UNLOCKED_IO])dnl AC_BEFORE([$0], [gl_ARGP])dnl AC_REQUIRE([AC_CANONICAL_HOST]) dnl _GNU_SOURCE is needed for pthread_rwlock_t on glibc systems. dnl AC_USE_SYSTEM_EXTENSIONS was introduced in autoconf 2.60 and obsoletes dnl AC_GNU_SOURCE. m4_ifdef([AC_USE_SYSTEM_EXTENSIONS], [AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS])], [AC_REQUIRE([AC_GNU_SOURCE])]) dnl Check for multithreading. m4_ifdef([gl_THREADLIB_DEFAULT_NO], [m4_divert_text([DEFAULTS], [gl_use_threads_default=no])], [m4_divert_text([DEFAULTS], [gl_use_threads_default=])]) AC_ARG_ENABLE([threads], AC_HELP_STRING([--enable-threads={posix|solaris|pth|windows}], [specify multithreading API])m4_ifdef([gl_THREADLIB_DEFAULT_NO], [], [ AC_HELP_STRING([--disable-threads], [build without multithread safety])]), [gl_use_threads=$enableval], [if test -n "$gl_use_threads_default"; then gl_use_threads="$gl_use_threads_default" else changequote(,)dnl case "$host_os" in dnl Disable multithreading by default on OSF/1, because it interferes dnl with fork()/exec(): When msgexec is linked with -lpthread, its dnl child process gets an endless segmentation fault inside execvp(). dnl Disable multithreading by default on Cygwin 1.5.x, because it has dnl bugs that lead to endless loops or crashes. See dnl . osf*) gl_use_threads=no ;; cygwin*) case `uname -r` in 1.[0-5].*) gl_use_threads=no ;; *) gl_use_threads=yes ;; esac ;; *) gl_use_threads=yes ;; esac changequote([,])dnl fi ]) if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # For using : case "$host_os" in osf*) # On OSF/1, the compiler needs the flag -D_REENTRANT so that it # groks . cc also understands the flag -pthread, but # we don't use it because 1. gcc-2.95 doesn't understand -pthread, # 2. putting a flag into CPPFLAGS that has an effect on the linker # causes the AC_LINK_IFELSE test below to succeed unexpectedly, # leading to wrong values of LIBTHREAD and LTLIBTHREAD. CPPFLAGS="$CPPFLAGS -D_REENTRANT" ;; esac # Some systems optimize for single-threaded programs by default, and # need special flags to disable these optimizations. For example, the # definition of 'errno' in . case "$host_os" in aix* | freebsd*) CPPFLAGS="$CPPFLAGS -D_THREAD_SAFE" ;; solaris*) CPPFLAGS="$CPPFLAGS -D_REENTRANT" ;; esac fi ]) dnl The guts of gl_THREADLIB. Needs to be expanded only once. AC_DEFUN([gl_THREADLIB_BODY], [ AC_REQUIRE([gl_THREADLIB_EARLY_BODY]) gl_threads_api=none LIBTHREAD= LTLIBTHREAD= LIBMULTITHREAD= LTLIBMULTITHREAD= if test "$gl_use_threads" != no; then dnl Check whether the compiler and linker support weak declarations. AC_CACHE_CHECK([whether imported symbols can be declared weak], [gl_cv_have_weak], [gl_cv_have_weak=no dnl First, test whether the compiler accepts it syntactically. AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[extern void xyzzy (); #pragma weak xyzzy]], [[xyzzy();]])], [gl_cv_have_weak=maybe]) if test $gl_cv_have_weak = maybe; then dnl Second, test whether it actually works. On Cygwin 1.7.2, with dnl gcc 4.3, symbols declared weak always evaluate to the address 0. AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #pragma weak fputs int main () { return (fputs == NULL); }]])], [gl_cv_have_weak=yes], [gl_cv_have_weak=no], [dnl When cross-compiling, assume that only ELF platforms support dnl weak symbols. AC_EGREP_CPP([Extensible Linking Format], [#ifdef __ELF__ Extensible Linking Format #endif ], [gl_cv_have_weak="guessing yes"], [gl_cv_have_weak="guessing no"]) ]) fi dnl But when linking statically, weak symbols don't work. case " $LDFLAGS " in *" -static "*) gl_cv_have_weak=no ;; esac ]) if test "$gl_use_threads" = yes || test "$gl_use_threads" = posix; then # On OSF/1, the compiler needs the flag -pthread or -D_REENTRANT so that # it groks . It's added above, in gl_THREADLIB_EARLY_BODY. AC_CHECK_HEADER([pthread.h], [gl_have_pthread_h=yes], [gl_have_pthread_h=no]) if test "$gl_have_pthread_h" = yes; then # Other possible tests: # -lpthreads (FSU threads, PCthreads) # -lgthreads gl_have_pthread= # Test whether both pthread_mutex_lock and pthread_mutexattr_init exist # in libc. IRIX 6.5 has the first one in both libc and libpthread, but # the second one only in libpthread, and lock.c needs it. # # If -pthread works, prefer it to -lpthread, since Ubuntu 14.04 # needs -pthread for some reason. See: # https://lists.gnu.org/r/bug-gnulib/2014-09/msg00023.html save_LIBS=$LIBS for gl_pthread in '' '-pthread'; do LIBS="$LIBS $gl_pthread" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include pthread_mutex_t m; pthread_mutexattr_t ma; ]], [[pthread_mutex_lock (&m); pthread_mutexattr_init (&ma);]])], [gl_have_pthread=yes LIBTHREAD=$gl_pthread LTLIBTHREAD=$gl_pthread LIBMULTITHREAD=$gl_pthread LTLIBMULTITHREAD=$gl_pthread]) LIBS=$save_LIBS test -n "$gl_have_pthread" && break done # Test for libpthread by looking for pthread_kill. (Not pthread_self, # since it is defined as a macro on OSF/1.) if test -n "$gl_have_pthread" && test -z "$LIBTHREAD"; then # The program links fine without libpthread. But it may actually # need to link with libpthread in order to create multiple threads. AC_CHECK_LIB([pthread], [pthread_kill], [LIBMULTITHREAD=-lpthread LTLIBMULTITHREAD=-lpthread # On Solaris and HP-UX, most pthread functions exist also in libc. # Therefore pthread_in_use() needs to actually try to create a # thread: pthread_create from libc will fail, whereas # pthread_create will actually create a thread. # On Solaris 10 or newer, this test is no longer needed, because # libc contains the fully functional pthread functions. case "$host_os" in solaris | solaris2.[1-9] | solaris2.[1-9].* | hpux*) AC_DEFINE([PTHREAD_IN_USE_DETECTION_HARD], [1], [Define if the pthread_in_use() detection is hard.]) esac ]) elif test -z "$gl_have_pthread"; then # Some library is needed. Try libpthread and libc_r. AC_CHECK_LIB([pthread], [pthread_kill], [gl_have_pthread=yes LIBTHREAD=-lpthread LTLIBTHREAD=-lpthread LIBMULTITHREAD=-lpthread LTLIBMULTITHREAD=-lpthread]) if test -z "$gl_have_pthread"; then # For FreeBSD 4. AC_CHECK_LIB([c_r], [pthread_kill], [gl_have_pthread=yes LIBTHREAD=-lc_r LTLIBTHREAD=-lc_r LIBMULTITHREAD=-lc_r LTLIBMULTITHREAD=-lc_r]) fi fi if test -n "$gl_have_pthread"; then gl_threads_api=posix AC_DEFINE([USE_POSIX_THREADS], [1], [Define if the POSIX multithreading library can be used.]) if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then AC_DEFINE([USE_POSIX_THREADS_WEAK], [1], [Define if references to the POSIX multithreading library should be made weak.]) LIBTHREAD= LTLIBTHREAD= fi fi fi fi fi if test -z "$gl_have_pthread"; then if test "$gl_use_threads" = yes || test "$gl_use_threads" = solaris; then gl_have_solaristhread= gl_save_LIBS="$LIBS" LIBS="$LIBS -lthread" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[ #include #include ]], [[thr_self();]])], [gl_have_solaristhread=yes]) LIBS="$gl_save_LIBS" if test -n "$gl_have_solaristhread"; then gl_threads_api=solaris LIBTHREAD=-lthread LTLIBTHREAD=-lthread LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" AC_DEFINE([USE_SOLARIS_THREADS], [1], [Define if the old Solaris multithreading library can be used.]) if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then AC_DEFINE([USE_SOLARIS_THREADS_WEAK], [1], [Define if references to the old Solaris multithreading library should be made weak.]) LIBTHREAD= LTLIBTHREAD= fi fi fi fi if test "$gl_use_threads" = pth; then gl_save_CPPFLAGS="$CPPFLAGS" AC_LIB_LINKFLAGS([pth]) gl_have_pth= gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBPTH" AC_LINK_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[pth_self();]])], [gl_have_pth=yes]) LIBS="$gl_save_LIBS" if test -n "$gl_have_pth"; then gl_threads_api=pth LIBTHREAD="$LIBPTH" LTLIBTHREAD="$LTLIBPTH" LIBMULTITHREAD="$LIBTHREAD" LTLIBMULTITHREAD="$LTLIBTHREAD" AC_DEFINE([USE_PTH_THREADS], [1], [Define if the GNU Pth multithreading library can be used.]) if test -n "$LIBMULTITHREAD" || test -n "$LTLIBMULTITHREAD"; then if case "$gl_cv_have_weak" in *yes) true;; *) false;; esac; then AC_DEFINE([USE_PTH_THREADS_WEAK], [1], [Define if references to the GNU Pth multithreading library should be made weak.]) LIBTHREAD= LTLIBTHREAD= fi fi else CPPFLAGS="$gl_save_CPPFLAGS" fi fi if test -z "$gl_have_pthread"; then case "$gl_use_threads" in yes | windows | win32) # The 'win32' is for backward compatibility. if { case "$host_os" in mingw*) true;; *) false;; esac }; then gl_threads_api=windows AC_DEFINE([USE_WINDOWS_THREADS], [1], [Define if the native Windows multithreading API can be used.]) fi ;; esac fi fi AC_MSG_CHECKING([for multithread API to use]) AC_MSG_RESULT([$gl_threads_api]) AC_SUBST([LIBTHREAD]) AC_SUBST([LTLIBTHREAD]) AC_SUBST([LIBMULTITHREAD]) AC_SUBST([LTLIBMULTITHREAD]) ]) AC_DEFUN([gl_THREADLIB], [ AC_REQUIRE([gl_THREADLIB_EARLY]) AC_REQUIRE([gl_THREADLIB_BODY]) ]) dnl gl_DISABLE_THREADS dnl ------------------ dnl Sets the gl_THREADLIB default so that threads are not used by default. dnl The user can still override it at installation time, by using the dnl configure option '--enable-threads'. AC_DEFUN([gl_DISABLE_THREADS], [ m4_divert_text([INIT_PREPARE], [gl_use_threads_default=no]) ]) dnl Survey of platforms: dnl dnl Platform Available Compiler Supports test-lock dnl flavours option weak result dnl --------------- --------- --------- -------- --------- dnl Linux 2.4/glibc posix -lpthread Y OK dnl dnl GNU Hurd/glibc posix dnl dnl Ubuntu 14.04 posix -pthread Y OK dnl dnl FreeBSD 5.3 posix -lc_r Y dnl posix -lkse ? Y dnl posix -lpthread ? Y dnl posix -lthr Y dnl dnl FreeBSD 5.2 posix -lc_r Y dnl posix -lkse Y dnl posix -lthr Y dnl dnl FreeBSD 4.0,4.10 posix -lc_r Y OK dnl dnl NetBSD 1.6 -- dnl dnl OpenBSD 3.4 posix -lpthread Y OK dnl dnl Mac OS X 10.[123] posix -lpthread Y OK dnl dnl Solaris 7,8,9 posix -lpthread Y Sol 7,8: 0.0; Sol 9: OK dnl solaris -lthread Y Sol 7,8: 0.0; Sol 9: OK dnl dnl HP-UX 11 posix -lpthread N (cc) OK dnl Y (gcc) dnl dnl IRIX 6.5 posix -lpthread Y 0.5 dnl dnl AIX 4.3,5.1 posix -lpthread N AIX 4: 0.5; AIX 5: OK dnl dnl OSF/1 4.0,5.1 posix -pthread (cc) N OK dnl -lpthread (gcc) Y dnl dnl Cygwin posix -lpthread Y OK dnl dnl Any of the above pth -lpth 0.0 dnl dnl Mingw windows N OK dnl dnl BeOS 5 -- dnl dnl The test-lock result shows what happens if in test-lock.c EXPLICIT_YIELD is dnl turned off: dnl OK if all three tests terminate OK, dnl 0.5 if the first test terminates OK but the second one loops endlessly, dnl 0.0 if the first test already loops endlessly. gnuastro-0.5/bootstrapped/m4/thread.m40000644000175000017500000000076113217200022014671 00000000000000# thread.m4 serial 3 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_THREAD], [ AC_REQUIRE([gl_THREADLIB]) if test $gl_threads_api = posix; then gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" AC_CHECK_FUNCS([pthread_atfork]) LIBS="$gl_save_LIBS" fi ]) gnuastro-0.5/bootstrapped/m4/sysexits.m40000644000175000017500000000237313217200022015316 00000000000000# sysexits.m4 serial 6 dnl Copyright (C) 2003, 2005, 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_SYSEXITS], [ AC_CHECK_HEADERS_ONCE([sysexits.h]) if test $ac_cv_header_sysexits_h = yes; then HAVE_SYSEXITS_H=1 gl_CHECK_NEXT_HEADERS([sysexits.h]) AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[switch (0) { case EX_OK: case EX_USAGE: case EX_DATAERR: case EX_NOINPUT: case EX_NOUSER: case EX_NOHOST: case EX_UNAVAILABLE: case EX_SOFTWARE: case EX_OSERR: case EX_OSFILE: case EX_CANTCREAT: case EX_IOERR: case EX_TEMPFAIL: case EX_PROTOCOL: case EX_NOPERM: case EX_CONFIG: break; } ]])], [SYSEXITS_H=], [SYSEXITS_H=sysexits.h]) else HAVE_SYSEXITS_H=0 SYSEXITS_H=sysexits.h fi AC_SUBST([HAVE_SYSEXITS_H]) AC_SUBST([SYSEXITS_H]) AM_CONDITIONAL([GL_GENERATE_SYSEXITS_H], [test -n "$SYSEXITS_H"]) ]) gnuastro-0.5/bootstrapped/m4/sys_uio_h.m40000644000175000017500000000165413217200022015425 00000000000000# sys_uio_h.m4 serial 1 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_HEADER_SYS_UIO], [ AC_REQUIRE([gl_SYS_UIO_H_DEFAULTS]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([sys/uio.h]) if test $ac_cv_header_sys_uio_h = yes; then HAVE_SYS_UIO_H=1 else HAVE_SYS_UIO_H=0 fi AC_SUBST([HAVE_SYS_UIO_H]) ]) AC_DEFUN([gl_SYS_UIO_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_UIO_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_UIO_H_DEFAULTS], [ ]) gnuastro-0.5/bootstrapped/m4/sys_types_h.m40000644000175000017500000000337313217200022015775 00000000000000# sys_types_h.m4 serial 9 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_SYS_TYPES_H], [ dnl Use sane struct stat types in OpenVMS 8.2 and later. AC_DEFINE([_USE_STD_STAT], 1, [For standard stat data types on VMS.]) AC_REQUIRE([gl_SYS_TYPES_H_DEFAULTS]) gl_NEXT_HEADERS([sys/types.h]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) dnl Ensure the type mode_t gets defined. AC_REQUIRE([AC_TYPE_MODE_T]) dnl Whether to override the 'off_t' type. AC_REQUIRE([gl_TYPE_OFF_T]) dnl Whether to override the 'dev_t' and 'ino_t' types. m4_ifdef([gl_WINDOWS_STAT_INODES], [ AC_REQUIRE([gl_WINDOWS_STAT_INODES]) ], [ WINDOWS_STAT_INODES=0 ]) AC_SUBST([WINDOWS_STAT_INODES]) ]) AC_DEFUN([gl_SYS_TYPES_H_DEFAULTS], [ ]) # This works around a buggy version in autoconf <= 2.69. # See m4_version_prereq([2.70], [], [ # This is taken from the following Autoconf patch: # https://git.savannah.gnu.org/cgit/autoconf.git/commit/?id=e17a30e987d7ee695fb4294a82d987ec3dc9b974 m4_undefine([AC_HEADER_MAJOR]) AC_DEFUN([AC_HEADER_MAJOR], [AC_CHECK_HEADERS_ONCE([sys/types.h]) AC_CHECK_HEADER([sys/mkdev.h], [AC_DEFINE([MAJOR_IN_MKDEV], [1], [Define to 1 if `major', `minor', and `makedev' are declared in .])]) if test $ac_cv_header_sys_mkdev_h = no; then AC_CHECK_HEADER([sys/sysmacros.h], [AC_DEFINE([MAJOR_IN_SYSMACROS], [1], [Define to 1 if `major', `minor', and `makedev' are declared in .])]) fi ]) ]) gnuastro-0.5/bootstrapped/m4/sys_time_h.m40000644000175000017500000000734113217200022015566 00000000000000# Configure a replacement for . # serial 9 # Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert and Martin Lambers. AC_DEFUN([gl_HEADER_SYS_TIME_H], [ dnl Use AC_REQUIRE here, so that the REPLACE_GETTIMEOFDAY=0 statement dnl below is expanded once only, before all REPLACE_GETTIMEOFDAY=1 dnl statements that occur in other macros. AC_REQUIRE([gl_HEADER_SYS_TIME_H_BODY]) ]) AC_DEFUN([gl_HEADER_SYS_TIME_H_BODY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_SYS_TIME_H_DEFAULTS]) AC_CHECK_HEADERS_ONCE([sys/time.h]) gl_CHECK_NEXT_HEADERS([sys/time.h]) if test $ac_cv_header_sys_time_h != yes; then HAVE_SYS_TIME_H=0 fi dnl On native Windows with MSVC, 'struct timeval' is defined in dnl only. So include that header in the list. gl_PREREQ_SYS_H_WINSOCK2 AC_CACHE_CHECK([for struct timeval], [gl_cv_sys_struct_timeval], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif ]], [[static struct timeval x; x.tv_sec = x.tv_usec;]])], [gl_cv_sys_struct_timeval=yes], [gl_cv_sys_struct_timeval=no]) ]) if test $gl_cv_sys_struct_timeval != yes; then HAVE_STRUCT_TIMEVAL=0 else dnl On native Windows with a 64-bit 'time_t', 'struct timeval' is defined dnl (in and for mingw64, in only dnl for MSVC) with a tv_sec field of type 'long' (32-bit!), which is dnl smaller than the 'time_t' type mandated by POSIX. dnl On OpenBSD 5.1 amd64, tv_sec is 64 bits and time_t 32 bits, but dnl that is good enough. AC_CACHE_CHECK([for wide-enough struct timeval.tv_sec member], [gl_cv_sys_struct_timeval_tv_sec], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#if HAVE_SYS_TIME_H #include #endif #include #if HAVE_WINSOCK2_H # include #endif ]], [[static struct timeval x; typedef int verify_tv_sec_type[ sizeof (time_t) <= sizeof x.tv_sec ? 1 : -1 ]; ]])], [gl_cv_sys_struct_timeval_tv_sec=yes], [gl_cv_sys_struct_timeval_tv_sec=no]) ]) if test $gl_cv_sys_struct_timeval_tv_sec != yes; then REPLACE_STRUCT_TIMEVAL=1 fi fi dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ #if HAVE_SYS_TIME_H # include #endif #include ]], [gettimeofday]) ]) AC_DEFUN([gl_SYS_TIME_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_SYS_TIME_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_HEADER_SYS_TIME_H_DEFAULTS], [ GNULIB_GETTIMEOFDAY=0; AC_SUBST([GNULIB_GETTIMEOFDAY]) dnl Assume POSIX behavior unless another module says otherwise. HAVE_GETTIMEOFDAY=1; AC_SUBST([HAVE_GETTIMEOFDAY]) HAVE_STRUCT_TIMEVAL=1; AC_SUBST([HAVE_STRUCT_TIMEVAL]) HAVE_SYS_TIME_H=1; AC_SUBST([HAVE_SYS_TIME_H]) REPLACE_GETTIMEOFDAY=0; AC_SUBST([REPLACE_GETTIMEOFDAY]) REPLACE_STRUCT_TIMEVAL=0; AC_SUBST([REPLACE_STRUCT_TIMEVAL]) ]) gnuastro-0.5/bootstrapped/m4/sys_stat_h.m40000644000175000017500000000741013217200022015600 00000000000000# sys_stat_h.m4 serial 31 -*- Autoconf -*- dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Eric Blake. dnl Provide a GNU-like . AC_DEFUN([gl_HEADER_SYS_STAT_H], [ AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) dnl Check for broken stat macros. AC_REQUIRE([AC_HEADER_STAT]) gl_CHECK_NEXT_HEADERS([sys/stat.h]) dnl Ensure the type mode_t gets defined. AC_REQUIRE([AC_TYPE_MODE_T]) dnl Whether to enable precise timestamps in 'struct stat'. m4_ifdef([gl_WINDOWS_STAT_TIMESPEC], [ AC_REQUIRE([gl_WINDOWS_STAT_TIMESPEC]) ], [ WINDOWS_STAT_TIMESPEC=0 ]) AC_SUBST([WINDOWS_STAT_TIMESPEC]) dnl Whether to ensure that struct stat.st_size is 64-bit wide. m4_ifdef([gl_LARGEFILE], [ AC_REQUIRE([gl_LARGEFILE]) ], [ WINDOWS_64_BIT_ST_SIZE=0 ]) AC_SUBST([WINDOWS_64_BIT_ST_SIZE]) dnl Define types that are supposed to be defined in or dnl . AC_CHECK_TYPE([nlink_t], [], [AC_DEFINE([nlink_t], [int], [Define to the type of st_nlink in struct stat, or a supertype.])], [#include #include ]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [fchmodat fstat fstatat futimens lchmod lstat mkdirat mkfifo mkfifoat mknod mknodat stat utimensat]) ]) # gl_HEADER_SYS_STAT_H AC_DEFUN([gl_SYS_STAT_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_STAT_H_DEFAULTS], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) dnl for REPLACE_FCHDIR GNULIB_FCHMODAT=0; AC_SUBST([GNULIB_FCHMODAT]) GNULIB_FSTAT=0; AC_SUBST([GNULIB_FSTAT]) GNULIB_FSTATAT=0; AC_SUBST([GNULIB_FSTATAT]) GNULIB_FUTIMENS=0; AC_SUBST([GNULIB_FUTIMENS]) GNULIB_LCHMOD=0; AC_SUBST([GNULIB_LCHMOD]) GNULIB_LSTAT=0; AC_SUBST([GNULIB_LSTAT]) GNULIB_MKDIRAT=0; AC_SUBST([GNULIB_MKDIRAT]) GNULIB_MKFIFO=0; AC_SUBST([GNULIB_MKFIFO]) GNULIB_MKFIFOAT=0; AC_SUBST([GNULIB_MKFIFOAT]) GNULIB_MKNOD=0; AC_SUBST([GNULIB_MKNOD]) GNULIB_MKNODAT=0; AC_SUBST([GNULIB_MKNODAT]) GNULIB_STAT=0; AC_SUBST([GNULIB_STAT]) GNULIB_UTIMENSAT=0; AC_SUBST([GNULIB_UTIMENSAT]) GNULIB_OVERRIDES_STRUCT_STAT=0; AC_SUBST([GNULIB_OVERRIDES_STRUCT_STAT]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FCHMODAT=1; AC_SUBST([HAVE_FCHMODAT]) HAVE_FSTATAT=1; AC_SUBST([HAVE_FSTATAT]) HAVE_FUTIMENS=1; AC_SUBST([HAVE_FUTIMENS]) HAVE_LCHMOD=1; AC_SUBST([HAVE_LCHMOD]) HAVE_LSTAT=1; AC_SUBST([HAVE_LSTAT]) HAVE_MKDIRAT=1; AC_SUBST([HAVE_MKDIRAT]) HAVE_MKFIFO=1; AC_SUBST([HAVE_MKFIFO]) HAVE_MKFIFOAT=1; AC_SUBST([HAVE_MKFIFOAT]) HAVE_MKNOD=1; AC_SUBST([HAVE_MKNOD]) HAVE_MKNODAT=1; AC_SUBST([HAVE_MKNODAT]) HAVE_UTIMENSAT=1; AC_SUBST([HAVE_UTIMENSAT]) REPLACE_FSTAT=0; AC_SUBST([REPLACE_FSTAT]) REPLACE_FSTATAT=0; AC_SUBST([REPLACE_FSTATAT]) REPLACE_FUTIMENS=0; AC_SUBST([REPLACE_FUTIMENS]) REPLACE_LSTAT=0; AC_SUBST([REPLACE_LSTAT]) REPLACE_MKDIR=0; AC_SUBST([REPLACE_MKDIR]) REPLACE_MKFIFO=0; AC_SUBST([REPLACE_MKFIFO]) REPLACE_MKNOD=0; AC_SUBST([REPLACE_MKNOD]) REPLACE_STAT=0; AC_SUBST([REPLACE_STAT]) REPLACE_UTIMENSAT=0; AC_SUBST([REPLACE_UTIMENSAT]) ]) gnuastro-0.5/bootstrapped/m4/sys_socket_h.m40000644000175000017500000001416313217200022016120 00000000000000# sys_socket_h.m4 serial 23 dnl Copyright (C) 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Simon Josefsson. AC_DEFUN([gl_HEADER_SYS_SOCKET], [ AC_REQUIRE([gl_SYS_SOCKET_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl On OSF/1, the functions recv(), send(), recvfrom(), sendto() have dnl old-style declarations (with return type 'int' instead of 'ssize_t') dnl unless _POSIX_PII_SOCKET is defined. case "$host_os" in osf*) AC_DEFINE([_POSIX_PII_SOCKET], [1], [Define to 1 in order to get the POSIX compatible declarations of socket functions.]) ;; esac AC_CACHE_CHECK([whether is self-contained], [gl_cv_header_sys_socket_h_selfcontained], [ AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[]])], [gl_cv_header_sys_socket_h_selfcontained=yes], [gl_cv_header_sys_socket_h_selfcontained=no]) ]) if test $gl_cv_header_sys_socket_h_selfcontained = yes; then dnl If the shutdown function exists, should define dnl SHUT_RD, SHUT_WR, SHUT_RDWR. AC_CHECK_FUNCS([shutdown]) if test $ac_cv_func_shutdown = yes; then AC_CACHE_CHECK([whether defines the SHUT_* macros], [gl_cv_header_sys_socket_h_shut], [ AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[int a[] = { SHUT_RD, SHUT_WR, SHUT_RDWR };]])], [gl_cv_header_sys_socket_h_shut=yes], [gl_cv_header_sys_socket_h_shut=no]) ]) if test $gl_cv_header_sys_socket_h_shut = no; then SYS_SOCKET_H='sys/socket.h' fi fi fi # We need to check for ws2tcpip.h now. gl_PREREQ_SYS_H_SOCKET AC_CHECK_TYPES([struct sockaddr_storage, sa_family_t],,,[ /* sys/types.h is not needed according to POSIX, but the sys/socket.h in i386-unknown-freebsd4.10 and powerpc-apple-darwin5.5 required it. */ #include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif ]) if test $ac_cv_type_struct_sockaddr_storage = no; then HAVE_STRUCT_SOCKADDR_STORAGE=0 fi if test $ac_cv_type_sa_family_t = no; then HAVE_SA_FAMILY_T=0 fi if test $ac_cv_type_struct_sockaddr_storage != no; then AC_CHECK_MEMBERS([struct sockaddr_storage.ss_family], [], [HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY=0], [#include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif ]) fi if test $HAVE_STRUCT_SOCKADDR_STORAGE = 0 || test $HAVE_SA_FAMILY_T = 0 \ || test $HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = 0; then SYS_SOCKET_H='sys/socket.h' fi gl_PREREQ_SYS_H_WINSOCK2 dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Some systems require prerequisite headers. */ #include #include ]], [socket connect accept bind getpeername getsockname getsockopt listen recv send recvfrom sendto setsockopt shutdown accept4]) ]) AC_DEFUN([gl_PREREQ_SYS_H_SOCKET], [ dnl Check prerequisites of the replacement. AC_REQUIRE([gl_CHECK_SOCKET_HEADERS]) gl_CHECK_NEXT_HEADERS([sys/socket.h]) if test $ac_cv_header_sys_socket_h = yes; then HAVE_SYS_SOCKET_H=1 HAVE_WS2TCPIP_H=0 else HAVE_SYS_SOCKET_H=0 if test $ac_cv_header_ws2tcpip_h = yes; then HAVE_WS2TCPIP_H=1 else HAVE_WS2TCPIP_H=0 fi fi AC_SUBST([HAVE_SYS_SOCKET_H]) AC_SUBST([HAVE_WS2TCPIP_H]) ]) # Common prerequisites of the replacement and of the # replacement. # Sets and substitutes HAVE_WINSOCK2_H. AC_DEFUN([gl_PREREQ_SYS_H_WINSOCK2], [ m4_ifdef([gl_UNISTD_H_DEFAULTS], [AC_REQUIRE([gl_UNISTD_H_DEFAULTS])]) m4_ifdef([gl_SYS_IOCTL_H_DEFAULTS], [AC_REQUIRE([gl_SYS_IOCTL_H_DEFAULTS])]) AC_CHECK_HEADERS_ONCE([sys/socket.h]) if test $ac_cv_header_sys_socket_h != yes; then dnl We cannot use AC_CHECK_HEADERS_ONCE here, because that would make dnl the check for those headers unconditional; yet cygwin reports dnl that the headers are present but cannot be compiled (since on dnl cygwin, all socket information should come from sys/socket.h). AC_CHECK_HEADERS([winsock2.h]) fi if test "$ac_cv_header_winsock2_h" = yes; then HAVE_WINSOCK2_H=1 UNISTD_H_HAVE_WINSOCK2_H=1 SYS_IOCTL_H_HAVE_WINSOCK2_H=1 else HAVE_WINSOCK2_H=0 fi AC_SUBST([HAVE_WINSOCK2_H]) ]) AC_DEFUN([gl_SYS_SOCKET_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_SOCKET_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_SOCKET_H_DEFAULTS], [ GNULIB_SOCKET=0; AC_SUBST([GNULIB_SOCKET]) GNULIB_CONNECT=0; AC_SUBST([GNULIB_CONNECT]) GNULIB_ACCEPT=0; AC_SUBST([GNULIB_ACCEPT]) GNULIB_BIND=0; AC_SUBST([GNULIB_BIND]) GNULIB_GETPEERNAME=0; AC_SUBST([GNULIB_GETPEERNAME]) GNULIB_GETSOCKNAME=0; AC_SUBST([GNULIB_GETSOCKNAME]) GNULIB_GETSOCKOPT=0; AC_SUBST([GNULIB_GETSOCKOPT]) GNULIB_LISTEN=0; AC_SUBST([GNULIB_LISTEN]) GNULIB_RECV=0; AC_SUBST([GNULIB_RECV]) GNULIB_SEND=0; AC_SUBST([GNULIB_SEND]) GNULIB_RECVFROM=0; AC_SUBST([GNULIB_RECVFROM]) GNULIB_SENDTO=0; AC_SUBST([GNULIB_SENDTO]) GNULIB_SETSOCKOPT=0; AC_SUBST([GNULIB_SETSOCKOPT]) GNULIB_SHUTDOWN=0; AC_SUBST([GNULIB_SHUTDOWN]) GNULIB_ACCEPT4=0; AC_SUBST([GNULIB_ACCEPT4]) HAVE_STRUCT_SOCKADDR_STORAGE=1; AC_SUBST([HAVE_STRUCT_SOCKADDR_STORAGE]) HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY=1; AC_SUBST([HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY]) HAVE_SA_FAMILY_T=1; AC_SUBST([HAVE_SA_FAMILY_T]) HAVE_ACCEPT4=1; AC_SUBST([HAVE_ACCEPT4]) ]) gnuastro-0.5/bootstrapped/m4/sys_select_h.m40000644000175000017500000000671613217200022016114 00000000000000# sys_select_h.m4 serial 20 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_HEADER_SYS_SELECT], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_SYS_SELECT_H_DEFAULTS]) AC_CACHE_CHECK([whether is self-contained], [gl_cv_header_sys_select_h_selfcontained], [ dnl Test against two bugs: dnl 1. On many platforms, assumes prior inclusion of dnl . dnl 2. On OSF/1 4.0, provides only a forward declaration dnl of 'struct timeval', and no definition of this type. AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[struct timeval b;]])], [gl_cv_header_sys_select_h_selfcontained=yes], [gl_cv_header_sys_select_h_selfcontained=no]) dnl Test against another bug: dnl 3. On Solaris 10, provides an FD_ZERO implementation dnl that relies on memset(), but without including . if test $gl_cv_header_sys_select_h_selfcontained = yes; then AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[int memset; int bzero;]]) ], [AC_LINK_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[ #undef memset #define memset nonexistent_memset extern #ifdef __cplusplus "C" #endif void *memset (void *, int, unsigned long); #undef bzero #define bzero nonexistent_bzero extern #ifdef __cplusplus "C" #endif void bzero (void *, unsigned long); fd_set fds; FD_ZERO (&fds); ]]) ], [], [gl_cv_header_sys_select_h_selfcontained=no]) ]) fi ]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([sys/select.h]) if test $ac_cv_header_sys_select_h = yes; then HAVE_SYS_SELECT_H=1 else HAVE_SYS_SELECT_H=0 fi AC_SUBST([HAVE_SYS_SELECT_H]) gl_PREREQ_SYS_H_WINSOCK2 dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Some systems require prerequisite headers. */ #include #if !(defined __GLIBC__ && !defined __UCLIBC__) && HAVE_SYS_TIME_H # include #endif #include ]], [pselect select]) ]) AC_DEFUN([gl_SYS_SELECT_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_SELECT_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_SELECT_H_DEFAULTS], [ GNULIB_PSELECT=0; AC_SUBST([GNULIB_PSELECT]) GNULIB_SELECT=0; AC_SUBST([GNULIB_SELECT]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_PSELECT=1; AC_SUBST([HAVE_PSELECT]) REPLACE_PSELECT=0; AC_SUBST([REPLACE_PSELECT]) REPLACE_SELECT=0; AC_SUBST([REPLACE_SELECT]) ]) gnuastro-0.5/bootstrapped/m4/sys_ioctl_h.m40000644000175000017500000000460613217200022015743 00000000000000# sys_ioctl_h.m4 serial 10 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Bruno Haible. AC_DEFUN([gl_SYS_IOCTL_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_SYS_IOCTL_H_DEFAULTS]) AC_CHECK_HEADERS_ONCE([sys/ioctl.h]) if test $ac_cv_header_sys_ioctl_h = yes; then HAVE_SYS_IOCTL_H=1 dnl Test whether declares ioctl(), or whether some other dnl header file, such as or , is needed for that. AC_CACHE_CHECK([whether declares ioctl], [gl_cv_decl_ioctl_in_sys_ioctl_h], [dnl We cannot use AC_CHECK_DECL because it produces its own messages. AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [AC_INCLUDES_DEFAULT([#include ])], [(void) ioctl;])], [gl_cv_decl_ioctl_in_sys_ioctl_h=yes], [gl_cv_decl_ioctl_in_sys_ioctl_h=no]) ]) else HAVE_SYS_IOCTL_H=0 fi AC_SUBST([HAVE_SYS_IOCTL_H]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([sys/ioctl.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include /* Some platforms declare ioctl in the wrong header. */ #if !(defined __GLIBC__ && !defined __UCLIBC__) # include #endif ]], [ioctl]) ]) AC_DEFUN([gl_SYS_IOCTL_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SYS_IOCTL_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SYS_IOCTL_H_DEFAULTS], [ GNULIB_IOCTL=0; AC_SUBST([GNULIB_IOCTL]) dnl Assume proper GNU behavior unless another module says otherwise. SYS_IOCTL_H_HAVE_WINSOCK2_H=0; AC_SUBST([SYS_IOCTL_H_HAVE_WINSOCK2_H]) SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=0; AC_SUBST([SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS]) REPLACE_IOCTL=0; AC_SUBST([REPLACE_IOCTL]) ]) gnuastro-0.5/bootstrapped/m4/symlink.m40000644000175000017500000000347113217200022015111 00000000000000# serial 6 # See if we need to provide symlink replacement. dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Written by Eric Blake. AC_DEFUN([gl_FUNC_SYMLINK], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_FUNCS_ONCE([symlink]) dnl The best we can do on mingw is provide a dummy that always fails, so dnl that compilation can proceed with fewer ifdefs. On FreeBSD 7.2, AIX 7.1, dnl and Solaris 9, we want to fix a bug with trailing slash handling. if test $ac_cv_func_symlink = no; then HAVE_SYMLINK=0 else AC_CACHE_CHECK([whether symlink handles trailing slash correctly], [gl_cv_func_symlink_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[int result = 0; if (!symlink ("a", "conftest.link/")) result |= 1; if (symlink ("conftest.f", "conftest.lnk2")) result |= 2; else if (!symlink ("a", "conftest.lnk2/")) result |= 4; return result; ]])], [gl_cv_func_symlink_works=yes], [gl_cv_func_symlink_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_symlink_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_symlink_works="guessing no" ;; esac ]) rm -f conftest.f conftest.link conftest.lnk2]) case "$gl_cv_func_symlink_works" in *yes) ;; *) REPLACE_SYMLINK=1 ;; esac fi ]) gnuastro-0.5/bootstrapped/m4/strtok_r.m40000644000175000017500000000506013217200022015266 00000000000000# strtok_r.m4 serial 14 dnl Copyright (C) 2002-2004, 2006-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRTOK_R], [ dnl The strtok_r() declaration in lib/string.in.h uses 'restrict'. AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_FUNCS([strtok_r]) if test $ac_cv_func_strtok_r = yes; then HAVE_STRTOK_R=1 dnl glibc 2.7 has a bug in strtok_r that causes a segmentation fault dnl when the second argument to strtok_r is a constant string that has dnl exactly one byte and compiling with optimization. This bug is, for dnl example, present in the glibc 2.7-18 package in Debian "lenny". dnl See . AC_CACHE_CHECK([whether strtok_r works], [gl_cv_func_strtok_r_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM([[ #ifndef __OPTIMIZE__ # define __OPTIMIZE__ 1 #endif #undef __OPTIMIZE_SIZE__ #undef __NO_INLINE__ #include #include ]], [[static const char dummy[] = "\177\01a"; char delimiters[] = "xxxxxxxx"; char *save_ptr = (char *) dummy; strtok_r (delimiters, "x", &save_ptr); strtok_r (NULL, "x", &save_ptr); return 0; ]]) ], [gl_cv_func_strtok_r_works=yes], [gl_cv_func_strtok_r_works=no], [case "$host_os" in # Guess no on glibc systems. *-gnu*) gl_cv_func_strtok_r_works="guessing no" ;; # Guess yes on native Windows. mingw*) gl_cv_func_strtok_r_works="guessing yes" ;; *) gl_cv_func_strtok_r_works="guessing yes" ;; esac ]) ]) case "$gl_cv_func_strtok_r_works" in *no) dnl We could set REPLACE_STRTOK_R=1 here, but it's only the macro dnl version in which is wrong. The code compiled dnl into libc is fine. UNDEFINE_STRTOK_R=1 ;; esac else HAVE_STRTOK_R=0 fi AC_CHECK_DECLS_ONCE([strtok_r]) if test $ac_cv_have_decl_strtok_r = no; then HAVE_DECL_STRTOK_R=0 fi ]) # Prerequisites of lib/strtok_r.c. AC_DEFUN([gl_PREREQ_STRTOK_R], [ : ]) gnuastro-0.5/bootstrapped/m4/strtod.m40000644000175000017500000001016113217200022014734 00000000000000# strtod.m4 serial 23 dnl Copyright (C) 2002-2003, 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRTOD], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles m4_ifdef([gl_FUNC_STRTOD_OBSOLETE], [ dnl Test whether strtod is declared. dnl Don't call AC_FUNC_STRTOD, because it does not have the right guess dnl when cross-compiling. dnl Don't call AC_CHECK_FUNCS([strtod]) because it would collide with the dnl ac_cv_func_strtod variable set by the AC_FUNC_STRTOD macro. AC_CHECK_DECLS_ONCE([strtod]) if test $ac_cv_have_decl_strtod != yes; then HAVE_STRTOD=0 fi ]) if test $HAVE_STRTOD = 1; then AC_CACHE_CHECK([whether strtod obeys C99], [gl_cv_func_strtod_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include #include /* Compare two numbers with ==. This is a separate function because IRIX 6.5 "cc -O" miscompiles an 'x == x' test. */ static int numeric_equal (double x, double y) { return x == y; } ]], [[ int result = 0; { /* In some old versions of Linux (2000 or before), strtod mis-parses strings with leading '+'. */ const char *string = " +69"; char *term; double value = strtod (string, &term); if (value != 69 || term != (string + 4)) result |= 1; } { /* Under Solaris 2.4, strtod returns the wrong value for the terminating character under some conditions. */ const char *string = "NaN"; char *term; strtod (string, &term); if (term != string && *(term - 1) == 0) result |= 2; } { /* Older glibc and Cygwin mis-parse "-0x". */ const char *string = "-0x"; char *term; double value = strtod (string, &term); double zero = 0.0; if (1.0 / value != -1.0 / zero || term != (string + 2)) result |= 4; } { /* Many platforms do not parse hex floats. */ const char *string = "0XaP+1"; char *term; double value = strtod (string, &term); if (value != 20.0 || term != (string + 6)) result |= 8; } { /* Many platforms do not parse infinities. HP-UX 11.31 parses inf, but mistakenly sets errno. */ const char *string = "inf"; char *term; double value; errno = 0; value = strtod (string, &term); if (value != HUGE_VAL || term != (string + 3) || errno) result |= 16; } { /* glibc 2.7 and cygwin 1.5.24 misparse "nan()". */ const char *string = "nan()"; char *term; double value = strtod (string, &term); if (numeric_equal (value, value) || term != (string + 5)) result |= 32; } { /* darwin 10.6.1 misparses "nan(". */ const char *string = "nan("; char *term; double value = strtod (string, &term); if (numeric_equal (value, value) || term != (string + 3)) result |= 64; } return result; ]])], [gl_cv_func_strtod_works=yes], [gl_cv_func_strtod_works=no], [dnl The last known bugs in glibc strtod(), as of this writing, dnl were fixed in version 2.8 AC_EGREP_CPP([Lucky user], [ #include #ifdef __GNU_LIBRARY__ #if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 8) || (__GLIBC__ > 2)) \ && !defined __UCLIBC__ Lucky user #endif #endif ], [gl_cv_func_strtod_works="guessing yes"], [case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_func_strtod_works="guessing yes" ;; *) gl_cv_func_strtod_works="guessing no" ;; esac ]) ]) ]) case "$gl_cv_func_strtod_works" in *yes) ;; *) REPLACE_STRTOD=1 ;; esac fi ]) # Prerequisites of lib/strtod.c. AC_DEFUN([gl_PREREQ_STRTOD], [ AC_REQUIRE([gl_CHECK_LDEXP_NO_LIBM]) if test $gl_cv_func_ldexp_no_libm = yes; then AC_DEFINE([HAVE_LDEXP_IN_LIBC], [1], [Define if the ldexp function is available in libc.]) fi ]) gnuastro-0.5/bootstrapped/m4/strnlen.m40000644000175000017500000000156113217200022015106 00000000000000# strnlen.m4 serial 13 dnl Copyright (C) 2002-2003, 2005-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRNLEN], [ AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) dnl Persuade glibc to declare strnlen(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_DECLS_ONCE([strnlen]) if test $ac_cv_have_decl_strnlen = no; then HAVE_DECL_STRNLEN=0 else m4_pushdef([AC_LIBOBJ], [:]) dnl Note: AC_FUNC_STRNLEN does AC_LIBOBJ([strnlen]). AC_FUNC_STRNLEN m4_popdef([AC_LIBOBJ]) if test $ac_cv_func_strnlen_working = no; then REPLACE_STRNLEN=1 fi fi ]) # Prerequisites of lib/strnlen.c. AC_DEFUN([gl_PREREQ_STRNLEN], [:]) gnuastro-0.5/bootstrapped/m4/strndup.m40000644000175000017500000000327413217200022015123 00000000000000# strndup.m4 serial 22 dnl Copyright (C) 2002-2003, 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRNDUP], [ dnl Persuade glibc to declare strndup(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_DECLS_ONCE([strndup]) AC_CHECK_FUNCS_ONCE([strndup]) if test $ac_cv_have_decl_strndup = no; then HAVE_DECL_STRNDUP=0 fi if test $ac_cv_func_strndup = yes; then HAVE_STRNDUP=1 # AIX 4.3.3, AIX 5.1 have a function that fails to add the terminating '\0'. AC_CACHE_CHECK([for working strndup], [gl_cv_func_strndup_works], [AC_RUN_IFELSE([ AC_LANG_PROGRAM([[#include #include ]], [[ #if !HAVE_DECL_STRNDUP extern #ifdef __cplusplus "C" #endif char *strndup (const char *, size_t); #endif int result; char *s; s = strndup ("some longer string", 15); free (s); s = strndup ("shorter string", 13); result = s[13] != '\0'; free (s); return result;]])], [gl_cv_func_strndup_works=yes], [gl_cv_func_strndup_works=no], [ changequote(,)dnl case $host_os in aix | aix[3-6]*) gl_cv_func_strndup_works="guessing no";; *) gl_cv_func_strndup_works="guessing yes";; esac changequote([,])dnl ])]) case $gl_cv_func_strndup_works in *no) REPLACE_STRNDUP=1 ;; esac else HAVE_STRNDUP=0 fi ]) gnuastro-0.5/bootstrapped/m4/strings_h.m40000644000175000017500000000316313217200022015421 00000000000000# Configure a replacement for . # serial 6 # Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_HEADER_STRINGS_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_HEADER_STRINGS_H_BODY]) ]) AC_DEFUN([gl_HEADER_STRINGS_H_BODY], [ AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([strings.h]) if test $ac_cv_header_strings_h = yes; then HAVE_STRINGS_H=1 else HAVE_STRINGS_H=0 fi AC_SUBST([HAVE_STRINGS_H]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* Minix 3.1.8 has a bug: must be included before . */ #include #include ]], [ffs strcasecmp strncasecmp]) ]) AC_DEFUN([gl_STRINGS_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_HEADER_STRINGS_H_DEFAULTS], [ GNULIB_FFS=0; AC_SUBST([GNULIB_FFS]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FFS=1; AC_SUBST([HAVE_FFS]) HAVE_STRCASECMP=1; AC_SUBST([HAVE_STRCASECMP]) HAVE_DECL_STRNCASECMP=1; AC_SUBST([HAVE_DECL_STRNCASECMP]) ]) gnuastro-0.5/bootstrapped/m4/string_h.m40000644000175000017500000001311113217200022015230 00000000000000# Configure a GNU-like replacement for . # Copyright (C) 2007-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # serial 22 # Written by Paul Eggert. AC_DEFUN([gl_HEADER_STRING_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_HEADER_STRING_H_BODY]) ]) AC_DEFUN([gl_HEADER_STRING_H_BODY], [ AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) gl_NEXT_HEADERS([string.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, and which is not dnl guaranteed by C89. gl_WARN_ON_USE_PREPARE([[#include ]], [ffsl ffsll memmem mempcpy memrchr rawmemchr stpcpy stpncpy strchrnul strdup strncat strndup strnlen strpbrk strsep strcasestr strtok_r strerror_r strsignal strverscmp]) ]) AC_DEFUN([gl_STRING_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_HEADER_STRING_H_DEFAULTS], [ GNULIB_EXPLICIT_BZERO=0; AC_SUBST([GNULIB_EXPLICIT_BZERO]) GNULIB_FFSL=0; AC_SUBST([GNULIB_FFSL]) GNULIB_FFSLL=0; AC_SUBST([GNULIB_FFSLL]) GNULIB_MEMCHR=0; AC_SUBST([GNULIB_MEMCHR]) GNULIB_MEMMEM=0; AC_SUBST([GNULIB_MEMMEM]) GNULIB_MEMPCPY=0; AC_SUBST([GNULIB_MEMPCPY]) GNULIB_MEMRCHR=0; AC_SUBST([GNULIB_MEMRCHR]) GNULIB_RAWMEMCHR=0; AC_SUBST([GNULIB_RAWMEMCHR]) GNULIB_STPCPY=0; AC_SUBST([GNULIB_STPCPY]) GNULIB_STPNCPY=0; AC_SUBST([GNULIB_STPNCPY]) GNULIB_STRCHRNUL=0; AC_SUBST([GNULIB_STRCHRNUL]) GNULIB_STRDUP=0; AC_SUBST([GNULIB_STRDUP]) GNULIB_STRNCAT=0; AC_SUBST([GNULIB_STRNCAT]) GNULIB_STRNDUP=0; AC_SUBST([GNULIB_STRNDUP]) GNULIB_STRNLEN=0; AC_SUBST([GNULIB_STRNLEN]) GNULIB_STRPBRK=0; AC_SUBST([GNULIB_STRPBRK]) GNULIB_STRSEP=0; AC_SUBST([GNULIB_STRSEP]) GNULIB_STRSTR=0; AC_SUBST([GNULIB_STRSTR]) GNULIB_STRCASESTR=0; AC_SUBST([GNULIB_STRCASESTR]) GNULIB_STRTOK_R=0; AC_SUBST([GNULIB_STRTOK_R]) GNULIB_MBSLEN=0; AC_SUBST([GNULIB_MBSLEN]) GNULIB_MBSNLEN=0; AC_SUBST([GNULIB_MBSNLEN]) GNULIB_MBSCHR=0; AC_SUBST([GNULIB_MBSCHR]) GNULIB_MBSRCHR=0; AC_SUBST([GNULIB_MBSRCHR]) GNULIB_MBSSTR=0; AC_SUBST([GNULIB_MBSSTR]) GNULIB_MBSCASECMP=0; AC_SUBST([GNULIB_MBSCASECMP]) GNULIB_MBSNCASECMP=0; AC_SUBST([GNULIB_MBSNCASECMP]) GNULIB_MBSPCASECMP=0; AC_SUBST([GNULIB_MBSPCASECMP]) GNULIB_MBSCASESTR=0; AC_SUBST([GNULIB_MBSCASESTR]) GNULIB_MBSCSPN=0; AC_SUBST([GNULIB_MBSCSPN]) GNULIB_MBSPBRK=0; AC_SUBST([GNULIB_MBSPBRK]) GNULIB_MBSSPN=0; AC_SUBST([GNULIB_MBSSPN]) GNULIB_MBSSEP=0; AC_SUBST([GNULIB_MBSSEP]) GNULIB_MBSTOK_R=0; AC_SUBST([GNULIB_MBSTOK_R]) GNULIB_STRERROR=0; AC_SUBST([GNULIB_STRERROR]) GNULIB_STRERROR_R=0; AC_SUBST([GNULIB_STRERROR_R]) GNULIB_STRSIGNAL=0; AC_SUBST([GNULIB_STRSIGNAL]) GNULIB_STRVERSCMP=0; AC_SUBST([GNULIB_STRVERSCMP]) HAVE_MBSLEN=0; AC_SUBST([HAVE_MBSLEN]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_EXPLICIT_BZERO=1; AC_SUBST([HAVE_EXPLICIT_BZERO]) HAVE_FFSL=1; AC_SUBST([HAVE_FFSL]) HAVE_FFSLL=1; AC_SUBST([HAVE_FFSLL]) HAVE_MEMCHR=1; AC_SUBST([HAVE_MEMCHR]) HAVE_DECL_MEMMEM=1; AC_SUBST([HAVE_DECL_MEMMEM]) HAVE_MEMPCPY=1; AC_SUBST([HAVE_MEMPCPY]) HAVE_DECL_MEMRCHR=1; AC_SUBST([HAVE_DECL_MEMRCHR]) HAVE_RAWMEMCHR=1; AC_SUBST([HAVE_RAWMEMCHR]) HAVE_STPCPY=1; AC_SUBST([HAVE_STPCPY]) HAVE_STPNCPY=1; AC_SUBST([HAVE_STPNCPY]) HAVE_STRCHRNUL=1; AC_SUBST([HAVE_STRCHRNUL]) HAVE_DECL_STRDUP=1; AC_SUBST([HAVE_DECL_STRDUP]) HAVE_DECL_STRNDUP=1; AC_SUBST([HAVE_DECL_STRNDUP]) HAVE_DECL_STRNLEN=1; AC_SUBST([HAVE_DECL_STRNLEN]) HAVE_STRPBRK=1; AC_SUBST([HAVE_STRPBRK]) HAVE_STRSEP=1; AC_SUBST([HAVE_STRSEP]) HAVE_STRCASESTR=1; AC_SUBST([HAVE_STRCASESTR]) HAVE_DECL_STRTOK_R=1; AC_SUBST([HAVE_DECL_STRTOK_R]) HAVE_DECL_STRERROR_R=1; AC_SUBST([HAVE_DECL_STRERROR_R]) HAVE_DECL_STRSIGNAL=1; AC_SUBST([HAVE_DECL_STRSIGNAL]) HAVE_STRVERSCMP=1; AC_SUBST([HAVE_STRVERSCMP]) REPLACE_MEMCHR=0; AC_SUBST([REPLACE_MEMCHR]) REPLACE_MEMMEM=0; AC_SUBST([REPLACE_MEMMEM]) REPLACE_STPNCPY=0; AC_SUBST([REPLACE_STPNCPY]) REPLACE_STRCHRNUL=0; AC_SUBST([REPLACE_STRCHRNUL]) REPLACE_STRDUP=0; AC_SUBST([REPLACE_STRDUP]) REPLACE_STRNCAT=0; AC_SUBST([REPLACE_STRNCAT]) REPLACE_STRNDUP=0; AC_SUBST([REPLACE_STRNDUP]) REPLACE_STRNLEN=0; AC_SUBST([REPLACE_STRNLEN]) REPLACE_STRSTR=0; AC_SUBST([REPLACE_STRSTR]) REPLACE_STRCASESTR=0; AC_SUBST([REPLACE_STRCASESTR]) REPLACE_STRTOK_R=0; AC_SUBST([REPLACE_STRTOK_R]) REPLACE_STRERROR=0; AC_SUBST([REPLACE_STRERROR]) REPLACE_STRERROR_R=0; AC_SUBST([REPLACE_STRERROR_R]) REPLACE_STRSIGNAL=0; AC_SUBST([REPLACE_STRSIGNAL]) UNDEFINE_STRTOK_R=0; AC_SUBST([UNDEFINE_STRTOK_R]) ]) gnuastro-0.5/bootstrapped/m4/strerror_r.m40000644000175000017500000001506713217200022015632 00000000000000# strerror_r.m4 serial 19 dnl Copyright (C) 2002, 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRERROR_R], [ AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_REQUIRE([gl_FUNC_STRERROR_R_WORKS]) dnl Persuade Solaris to declare strerror_r(). AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) dnl Some systems don't declare strerror_r() if _THREAD_SAFE and _REENTRANT dnl are not defined. AC_CHECK_DECLS_ONCE([strerror_r]) if test $ac_cv_have_decl_strerror_r = no; then HAVE_DECL_STRERROR_R=0 fi if test $ac_cv_func_strerror_r = yes; then if test "$ERRNO_H:$REPLACE_STRERROR_0" = :0; then if test $gl_cv_func_strerror_r_posix_signature = yes; then case "$gl_cv_func_strerror_r_works" in dnl The system's strerror_r has bugs. Replace it. *no) REPLACE_STRERROR_R=1 ;; esac else dnl The system's strerror_r() has a wrong signature. Replace it. REPLACE_STRERROR_R=1 fi else dnl The system's strerror_r() cannot know about the new errno values we dnl add to , or any fix for strerror(0). Replace it. REPLACE_STRERROR_R=1 fi fi ]) # Prerequisites of lib/strerror_r.c. AC_DEFUN([gl_PREREQ_STRERROR_R], [ dnl glibc >= 2.3.4 and cygwin 1.7.9 have a function __xpg_strerror_r. AC_CHECK_FUNCS_ONCE([__xpg_strerror_r]) AC_CHECK_FUNCS_ONCE([catgets]) AC_CHECK_FUNCS_ONCE([snprintf]) ]) # Detect if strerror_r works, but without affecting whether a replacement # strerror_r will be used. AC_DEFUN([gl_FUNC_STRERROR_R_WORKS], [ AC_REQUIRE([gl_HEADER_ERRNO_H]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_FUNC_STRERROR_0]) AC_CHECK_FUNCS_ONCE([strerror_r]) if test $ac_cv_func_strerror_r = yes; then if test "$ERRNO_H:$REPLACE_STRERROR_0" = :0; then dnl The POSIX prototype is: int strerror_r (int, char *, size_t); dnl glibc, Cygwin: char *strerror_r (int, char *, size_t); dnl AIX 5.1, OSF/1 5.1: int strerror_r (int, char *, int); AC_CACHE_CHECK([for strerror_r with POSIX signature], [gl_cv_func_strerror_r_posix_signature], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int strerror_r (int, char *, size_t); ]], [])], [gl_cv_func_strerror_r_posix_signature=yes], [gl_cv_func_strerror_r_posix_signature=no]) ]) if test $gl_cv_func_strerror_r_posix_signature = yes; then dnl AIX 6.1 strerror_r fails by returning -1, not an error number. dnl HP-UX 11.31 strerror_r always fails when the buffer length argument dnl is less than 80. dnl FreeBSD 8.s strerror_r claims failure on 0 dnl Mac OS X 10.5 strerror_r treats 0 like -1 dnl Solaris 10 strerror_r corrupts errno on failure AC_CACHE_CHECK([whether strerror_r works], [gl_cv_func_strerror_r_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[int result = 0; char buf[79]; if (strerror_r (EACCES, buf, 0) < 0) result |= 1; errno = 0; if (strerror_r (EACCES, buf, sizeof buf) != 0) result |= 2; strcpy (buf, "Unknown"); if (strerror_r (0, buf, sizeof buf) != 0) result |= 4; if (errno) result |= 8; if (strstr (buf, "nknown") || strstr (buf, "ndefined")) result |= 0x10; errno = 0; *buf = 0; if (strerror_r (-3, buf, sizeof buf) < 0) result |= 0x20; if (errno) result |= 0x40; if (!*buf) result |= 0x80; return result; ]])], [gl_cv_func_strerror_r_works=yes], [gl_cv_func_strerror_r_works=no], [ changequote(,)dnl case "$host_os" in # Guess no on AIX. aix*) gl_cv_func_strerror_r_works="guessing no";; # Guess no on HP-UX. hpux*) gl_cv_func_strerror_r_works="guessing no";; # Guess no on BSD variants. *bsd*) gl_cv_func_strerror_r_works="guessing no";; # Guess yes otherwise. *) gl_cv_func_strerror_r_works="guessing yes";; esac changequote([,])dnl ]) ]) else dnl The system's strerror() has a wrong signature. dnl glibc >= 2.3.4 and cygwin 1.7.9 have a function __xpg_strerror_r. AC_CHECK_FUNCS_ONCE([__xpg_strerror_r]) dnl In glibc < 2.14, __xpg_strerror_r does not populate buf on failure. dnl In cygwin < 1.7.10, __xpg_strerror_r clobbers strerror's buffer. if test $ac_cv_func___xpg_strerror_r = yes; then AC_CACHE_CHECK([whether __xpg_strerror_r works], [gl_cv_func_strerror_r_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include extern #ifdef __cplusplus "C" #endif int __xpg_strerror_r(int, char *, size_t); ]], [[int result = 0; char buf[256] = "^"; char copy[256]; char *str = strerror (-1); strcpy (copy, str); if (__xpg_strerror_r (-2, buf, 1) == 0) result |= 1; if (*buf) result |= 2; __xpg_strerror_r (-2, buf, 256); if (strcmp (str, copy)) result |= 4; return result; ]])], [gl_cv_func_strerror_r_works=yes], [gl_cv_func_strerror_r_works=no], [dnl Guess no on all platforms that have __xpg_strerror_r, dnl at least until fixed glibc and cygwin are more common. gl_cv_func_strerror_r_works="guessing no" ]) ]) fi fi fi fi ]) gnuastro-0.5/bootstrapped/m4/strerror.m40000644000175000017500000000641513217200022015306 00000000000000# strerror.m4 serial 18 dnl Copyright (C) 2002, 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRERROR], [ AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_REQUIRE([gl_HEADER_ERRNO_H]) AC_REQUIRE([gl_FUNC_STRERROR_0]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles m4_ifdef([gl_FUNC_STRERROR_R_WORKS], [ AC_REQUIRE([gl_FUNC_STRERROR_R_WORKS]) ]) if test "$ERRNO_H:$REPLACE_STRERROR_0" = :0; then AC_CACHE_CHECK([for working strerror function], [gl_cv_func_working_strerror], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[if (!*strerror (-2)) return 1;]])], [gl_cv_func_working_strerror=yes], [gl_cv_func_working_strerror=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_working_strerror="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_working_strerror="guessing no" ;; esac ]) ]) case "$gl_cv_func_working_strerror" in *yes) ;; *) dnl The system's strerror() fails to return a string for out-of-range dnl integers. Replace it. REPLACE_STRERROR=1 ;; esac m4_ifdef([gl_FUNC_STRERROR_R_WORKS], [ dnl If the system's strerror_r or __xpg_strerror_r clobbers strerror's dnl buffer, we must replace strerror. case "$gl_cv_func_strerror_r_works" in *no) REPLACE_STRERROR=1 ;; esac ]) else dnl The system's strerror() cannot know about the new errno values we add dnl to , or any fix for strerror(0). Replace it. REPLACE_STRERROR=1 fi ]) dnl Detect if strerror(0) passes (that is, does not set errno, and does not dnl return a string that matches strerror(-1)). AC_DEFUN([gl_FUNC_STRERROR_0], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles REPLACE_STRERROR_0=0 AC_CACHE_CHECK([whether strerror(0) succeeds], [gl_cv_func_strerror_0_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[int result = 0; char *str; errno = 0; str = strerror (0); if (!*str) result |= 1; if (errno) result |= 2; if (strstr (str, "nknown") || strstr (str, "ndefined")) result |= 4; return result;]])], [gl_cv_func_strerror_0_works=yes], [gl_cv_func_strerror_0_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_strerror_0_works="guessing yes" ;; # Guess yes on native Windows. mingw*) gl_cv_func_strerror_0_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_strerror_0_works="guessing no" ;; esac ]) ]) case "$gl_cv_func_strerror_0_works" in *yes) ;; *) REPLACE_STRERROR_0=1 AC_DEFINE([REPLACE_STRERROR_0], [1], [Define to 1 if strerror(0) does not return a message implying success.]) ;; esac ]) gnuastro-0.5/bootstrapped/m4/strchrnul.m40000644000175000017500000000276613217200022015455 00000000000000# strchrnul.m4 serial 9 dnl Copyright (C) 2003, 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STRCHRNUL], [ dnl Persuade glibc to declare strchrnul(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_FUNCS([strchrnul]) if test $ac_cv_func_strchrnul = no; then HAVE_STRCHRNUL=0 else AC_CACHE_CHECK([whether strchrnul works], [gl_cv_func_strchrnul_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include /* for strchrnul */ ]], [[const char *buf = "a"; return strchrnul (buf, 'b') != buf + 1; ]])], [gl_cv_func_strchrnul_works=yes], [gl_cv_func_strchrnul_works=no], [dnl Cygwin 1.7.9 introduced strchrnul, but it was broken until 1.7.10 AC_EGREP_CPP([Lucky user], [ #if defined __CYGWIN__ #include #if CYGWIN_VERSION_DLL_COMBINED > CYGWIN_VERSION_DLL_MAKE_COMBINED (1007, 9) Lucky user #endif #else Lucky user #endif ], [gl_cv_func_strchrnul_works="guessing yes"], [gl_cv_func_strchrnul_works="guessing no"]) ]) ]) case "$gl_cv_func_strchrnul_works" in *yes) ;; *) REPLACE_STRCHRNUL=1 ;; esac fi ]) # Prerequisites of lib/strchrnul.c. AC_DEFUN([gl_PREREQ_STRCHRNUL], [:]) gnuastro-0.5/bootstrapped/m4/strcase.m40000644000175000017500000000201213217200022015055 00000000000000# strcase.m4 serial 11 dnl Copyright (C) 2002, 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STRCASE], [ gl_FUNC_STRCASECMP gl_FUNC_STRNCASECMP ]) AC_DEFUN([gl_FUNC_STRCASECMP], [ AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) AC_CHECK_FUNCS([strcasecmp]) if test $ac_cv_func_strcasecmp = no; then HAVE_STRCASECMP=0 fi ]) AC_DEFUN([gl_FUNC_STRNCASECMP], [ AC_REQUIRE([gl_HEADER_STRINGS_H_DEFAULTS]) AC_CHECK_FUNCS([strncasecmp]) if test $ac_cv_func_strncasecmp = yes; then HAVE_STRNCASECMP=1 else HAVE_STRNCASECMP=0 fi AC_CHECK_DECLS([strncasecmp]) if test $ac_cv_have_decl_strncasecmp = no; then HAVE_DECL_STRNCASECMP=0 fi ]) # Prerequisites of lib/strcasecmp.c. AC_DEFUN([gl_PREREQ_STRCASECMP], [ : ]) # Prerequisites of lib/strncasecmp.c. AC_DEFUN([gl_PREREQ_STRNCASECMP], [ : ]) gnuastro-0.5/bootstrapped/m4/stdlib_h.m40000644000175000017500000001375013217200022015214 00000000000000# stdlib_h.m4 serial 44 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STDLIB_H], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) gl_NEXT_HEADERS([stdlib.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, and which is not dnl guaranteed by C89. gl_WARN_ON_USE_PREPARE([[#include #if HAVE_SYS_LOADAVG_H # include #endif #if HAVE_RANDOM_H # include #endif ]], [_Exit atoll canonicalize_file_name getloadavg getsubopt grantpt initstate initstate_r mkdtemp mkostemp mkostemps mkstemp mkstemps posix_openpt ptsname ptsname_r qsort_r random random_r reallocarray realpath rpmatch secure_getenv setenv setstate setstate_r srandom srandom_r strtod strtoll strtoull unlockpt unsetenv]) ]) AC_DEFUN([gl_STDLIB_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_STDLIB_H_DEFAULTS], [ GNULIB__EXIT=0; AC_SUBST([GNULIB__EXIT]) GNULIB_ATOLL=0; AC_SUBST([GNULIB_ATOLL]) GNULIB_CALLOC_POSIX=0; AC_SUBST([GNULIB_CALLOC_POSIX]) GNULIB_CANONICALIZE_FILE_NAME=0; AC_SUBST([GNULIB_CANONICALIZE_FILE_NAME]) GNULIB_GETLOADAVG=0; AC_SUBST([GNULIB_GETLOADAVG]) GNULIB_GETSUBOPT=0; AC_SUBST([GNULIB_GETSUBOPT]) GNULIB_GRANTPT=0; AC_SUBST([GNULIB_GRANTPT]) GNULIB_MALLOC_POSIX=0; AC_SUBST([GNULIB_MALLOC_POSIX]) GNULIB_MBTOWC=0; AC_SUBST([GNULIB_MBTOWC]) GNULIB_MKDTEMP=0; AC_SUBST([GNULIB_MKDTEMP]) GNULIB_MKOSTEMP=0; AC_SUBST([GNULIB_MKOSTEMP]) GNULIB_MKOSTEMPS=0; AC_SUBST([GNULIB_MKOSTEMPS]) GNULIB_MKSTEMP=0; AC_SUBST([GNULIB_MKSTEMP]) GNULIB_MKSTEMPS=0; AC_SUBST([GNULIB_MKSTEMPS]) GNULIB_POSIX_OPENPT=0; AC_SUBST([GNULIB_POSIX_OPENPT]) GNULIB_PTSNAME=0; AC_SUBST([GNULIB_PTSNAME]) GNULIB_PTSNAME_R=0; AC_SUBST([GNULIB_PTSNAME_R]) GNULIB_PUTENV=0; AC_SUBST([GNULIB_PUTENV]) GNULIB_QSORT_R=0; AC_SUBST([GNULIB_QSORT_R]) GNULIB_RANDOM=0; AC_SUBST([GNULIB_RANDOM]) GNULIB_RANDOM_R=0; AC_SUBST([GNULIB_RANDOM_R]) GNULIB_REALLOCARRAY=0; AC_SUBST([GNULIB_REALLOCARRAY]) GNULIB_REALLOC_POSIX=0; AC_SUBST([GNULIB_REALLOC_POSIX]) GNULIB_REALPATH=0; AC_SUBST([GNULIB_REALPATH]) GNULIB_RPMATCH=0; AC_SUBST([GNULIB_RPMATCH]) GNULIB_SECURE_GETENV=0; AC_SUBST([GNULIB_SECURE_GETENV]) GNULIB_SETENV=0; AC_SUBST([GNULIB_SETENV]) GNULIB_STRTOD=0; AC_SUBST([GNULIB_STRTOD]) GNULIB_STRTOLL=0; AC_SUBST([GNULIB_STRTOLL]) GNULIB_STRTOULL=0; AC_SUBST([GNULIB_STRTOULL]) GNULIB_SYSTEM_POSIX=0; AC_SUBST([GNULIB_SYSTEM_POSIX]) GNULIB_UNLOCKPT=0; AC_SUBST([GNULIB_UNLOCKPT]) GNULIB_UNSETENV=0; AC_SUBST([GNULIB_UNSETENV]) GNULIB_WCTOMB=0; AC_SUBST([GNULIB_WCTOMB]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE__EXIT=1; AC_SUBST([HAVE__EXIT]) HAVE_ATOLL=1; AC_SUBST([HAVE_ATOLL]) HAVE_CANONICALIZE_FILE_NAME=1; AC_SUBST([HAVE_CANONICALIZE_FILE_NAME]) HAVE_DECL_GETLOADAVG=1; AC_SUBST([HAVE_DECL_GETLOADAVG]) HAVE_GETSUBOPT=1; AC_SUBST([HAVE_GETSUBOPT]) HAVE_GRANTPT=1; AC_SUBST([HAVE_GRANTPT]) HAVE_DECL_INITSTATE=1; AC_SUBST([HAVE_DECL_INITSTATE]) HAVE_MKDTEMP=1; AC_SUBST([HAVE_MKDTEMP]) HAVE_MKOSTEMP=1; AC_SUBST([HAVE_MKOSTEMP]) HAVE_MKOSTEMPS=1; AC_SUBST([HAVE_MKOSTEMPS]) HAVE_MKSTEMP=1; AC_SUBST([HAVE_MKSTEMP]) HAVE_MKSTEMPS=1; AC_SUBST([HAVE_MKSTEMPS]) HAVE_POSIX_OPENPT=1; AC_SUBST([HAVE_POSIX_OPENPT]) HAVE_PTSNAME=1; AC_SUBST([HAVE_PTSNAME]) HAVE_PTSNAME_R=1; AC_SUBST([HAVE_PTSNAME_R]) HAVE_QSORT_R=1; AC_SUBST([HAVE_QSORT_R]) HAVE_RANDOM=1; AC_SUBST([HAVE_RANDOM]) HAVE_RANDOM_H=1; AC_SUBST([HAVE_RANDOM_H]) HAVE_RANDOM_R=1; AC_SUBST([HAVE_RANDOM_R]) HAVE_REALLOCARRAY=1; AC_SUBST([HAVE_REALLOCARRAY]) HAVE_REALPATH=1; AC_SUBST([HAVE_REALPATH]) HAVE_RPMATCH=1; AC_SUBST([HAVE_RPMATCH]) HAVE_SECURE_GETENV=1; AC_SUBST([HAVE_SECURE_GETENV]) HAVE_SETENV=1; AC_SUBST([HAVE_SETENV]) HAVE_DECL_SETENV=1; AC_SUBST([HAVE_DECL_SETENV]) HAVE_DECL_SETSTATE=1; AC_SUBST([HAVE_DECL_SETSTATE]) HAVE_STRTOD=1; AC_SUBST([HAVE_STRTOD]) HAVE_STRTOLL=1; AC_SUBST([HAVE_STRTOLL]) HAVE_STRTOULL=1; AC_SUBST([HAVE_STRTOULL]) HAVE_STRUCT_RANDOM_DATA=1; AC_SUBST([HAVE_STRUCT_RANDOM_DATA]) HAVE_SYS_LOADAVG_H=0; AC_SUBST([HAVE_SYS_LOADAVG_H]) HAVE_UNLOCKPT=1; AC_SUBST([HAVE_UNLOCKPT]) HAVE_DECL_UNSETENV=1; AC_SUBST([HAVE_DECL_UNSETENV]) REPLACE_CALLOC=0; AC_SUBST([REPLACE_CALLOC]) REPLACE_CANONICALIZE_FILE_NAME=0; AC_SUBST([REPLACE_CANONICALIZE_FILE_NAME]) REPLACE_MALLOC=0; AC_SUBST([REPLACE_MALLOC]) REPLACE_MBTOWC=0; AC_SUBST([REPLACE_MBTOWC]) REPLACE_MKSTEMP=0; AC_SUBST([REPLACE_MKSTEMP]) REPLACE_PTSNAME=0; AC_SUBST([REPLACE_PTSNAME]) REPLACE_PTSNAME_R=0; AC_SUBST([REPLACE_PTSNAME_R]) REPLACE_PUTENV=0; AC_SUBST([REPLACE_PUTENV]) REPLACE_QSORT_R=0; AC_SUBST([REPLACE_QSORT_R]) REPLACE_RANDOM_R=0; AC_SUBST([REPLACE_RANDOM_R]) REPLACE_REALLOC=0; AC_SUBST([REPLACE_REALLOC]) REPLACE_REALPATH=0; AC_SUBST([REPLACE_REALPATH]) REPLACE_SETENV=0; AC_SUBST([REPLACE_SETENV]) REPLACE_STRTOD=0; AC_SUBST([REPLACE_STRTOD]) REPLACE_UNSETENV=0; AC_SUBST([REPLACE_UNSETENV]) REPLACE_WCTOMB=0; AC_SUBST([REPLACE_WCTOMB]) ]) gnuastro-0.5/bootstrapped/m4/stdio_h.m40000644000175000017500000002525613217200022015061 00000000000000# stdio_h.m4 serial 48 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STDIO_H], [ AH_VERBATIM([MINGW_ANSI_STDIO], [/* Use GNU style printf and scanf. */ #ifndef __USE_MINGW_ANSI_STDIO # undef __USE_MINGW_ANSI_STDIO #endif ]) AC_DEFINE([__USE_MINGW_ANSI_STDIO]) AC_REQUIRE([gl_STDIO_H_DEFAULTS]) gl_NEXT_HEADERS([stdio.h]) dnl Determine whether __USE_MINGW_ANSI_STDIO makes printf and dnl inttypes.h behave like gnu instead of system; we must give our dnl printf wrapper the right attribute to match. AC_CACHE_CHECK([which flavor of printf attribute matches inttypes macros], [gl_cv_func_printf_attribute_flavor], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[ #define __STDC_FORMAT_MACROS 1 #include #include /* For non-mingw systems, compilation will trivially succeed. For mingw, compilation will succeed for older mingw (system printf, "I64d") and fail for newer mingw (gnu printf, "lld"). */ #if ((defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__) && \ (__GNUC__ > 4 || (__GNUC__ == 4 && __GNUC_MINOR__ >= 4)) extern char PRIdMAX_probe[sizeof PRIdMAX == sizeof "I64d" ? 1 : -1]; #endif ]])], [gl_cv_func_printf_attribute_flavor=system], [gl_cv_func_printf_attribute_flavor=gnu])]) if test "$gl_cv_func_printf_attribute_flavor" = gnu; then AC_DEFINE([GNULIB_PRINTF_ATTRIBUTE_FLAVOR_GNU], [1], [Define to 1 if printf and friends should be labeled with attribute "__gnu_printf__" instead of "__printf__"]) fi dnl No need to create extra modules for these functions. Everyone who uses dnl likely needs them. GNULIB_FSCANF=1 gl_MODULE_INDICATOR([fscanf]) GNULIB_SCANF=1 gl_MODULE_INDICATOR([scanf]) GNULIB_FGETC=1 GNULIB_GETC=1 GNULIB_GETCHAR=1 GNULIB_FGETS=1 GNULIB_FREAD=1 dnl This ifdef is necessary to avoid an error "missing file lib/stdio-read.c" dnl "expected source file, required through AC_LIBSOURCES, not found". It is dnl also an optimization, to avoid performing a configure check whose result dnl is not used. But it does not make the test of GNULIB_STDIO_H_NONBLOCKING dnl or GNULIB_NONBLOCKING redundant. m4_ifdef([gl_NONBLOCKING_IO], [ gl_NONBLOCKING_IO if test $gl_cv_have_nonblocking != yes; then REPLACE_STDIO_READ_FUNCS=1 AC_LIBOBJ([stdio-read]) fi ]) dnl No need to create extra modules for these functions. Everyone who uses dnl likely needs them. GNULIB_FPRINTF=1 GNULIB_PRINTF=1 GNULIB_VFPRINTF=1 GNULIB_VPRINTF=1 GNULIB_FPUTC=1 GNULIB_PUTC=1 GNULIB_PUTCHAR=1 GNULIB_FPUTS=1 GNULIB_PUTS=1 GNULIB_FWRITE=1 dnl This ifdef is necessary to avoid an error "missing file lib/stdio-write.c" dnl "expected source file, required through AC_LIBSOURCES, not found". It is dnl also an optimization, to avoid performing a configure check whose result dnl is not used. But it does not make the test of GNULIB_STDIO_H_SIGPIPE or dnl GNULIB_SIGPIPE redundant. m4_ifdef([gl_SIGNAL_SIGPIPE], [ gl_SIGNAL_SIGPIPE if test $gl_cv_header_signal_h_SIGPIPE != yes; then REPLACE_STDIO_WRITE_FUNCS=1 AC_LIBOBJ([stdio-write]) fi ]) dnl This ifdef is necessary to avoid an error "missing file lib/stdio-write.c" dnl "expected source file, required through AC_LIBSOURCES, not found". It is dnl also an optimization, to avoid performing a configure check whose result dnl is not used. But it does not make the test of GNULIB_STDIO_H_NONBLOCKING dnl or GNULIB_NONBLOCKING redundant. m4_ifdef([gl_NONBLOCKING_IO], [ gl_NONBLOCKING_IO if test $gl_cv_have_nonblocking != yes; then REPLACE_STDIO_WRITE_FUNCS=1 AC_LIBOBJ([stdio-write]) fi ]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, and which is not dnl guaranteed by both C89 and C11. gl_WARN_ON_USE_PREPARE([[#include ]], [dprintf fpurge fseeko ftello getdelim getline gets pclose popen renameat snprintf tmpfile vdprintf vsnprintf]) ]) AC_DEFUN([gl_STDIO_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_STDIO_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_STDIO_H_DEFAULTS], [ GNULIB_DPRINTF=0; AC_SUBST([GNULIB_DPRINTF]) GNULIB_FCLOSE=0; AC_SUBST([GNULIB_FCLOSE]) GNULIB_FDOPEN=0; AC_SUBST([GNULIB_FDOPEN]) GNULIB_FFLUSH=0; AC_SUBST([GNULIB_FFLUSH]) GNULIB_FGETC=0; AC_SUBST([GNULIB_FGETC]) GNULIB_FGETS=0; AC_SUBST([GNULIB_FGETS]) GNULIB_FOPEN=0; AC_SUBST([GNULIB_FOPEN]) GNULIB_FPRINTF=0; AC_SUBST([GNULIB_FPRINTF]) GNULIB_FPRINTF_POSIX=0; AC_SUBST([GNULIB_FPRINTF_POSIX]) GNULIB_FPURGE=0; AC_SUBST([GNULIB_FPURGE]) GNULIB_FPUTC=0; AC_SUBST([GNULIB_FPUTC]) GNULIB_FPUTS=0; AC_SUBST([GNULIB_FPUTS]) GNULIB_FREAD=0; AC_SUBST([GNULIB_FREAD]) GNULIB_FREOPEN=0; AC_SUBST([GNULIB_FREOPEN]) GNULIB_FSCANF=0; AC_SUBST([GNULIB_FSCANF]) GNULIB_FSEEK=0; AC_SUBST([GNULIB_FSEEK]) GNULIB_FSEEKO=0; AC_SUBST([GNULIB_FSEEKO]) GNULIB_FTELL=0; AC_SUBST([GNULIB_FTELL]) GNULIB_FTELLO=0; AC_SUBST([GNULIB_FTELLO]) GNULIB_FWRITE=0; AC_SUBST([GNULIB_FWRITE]) GNULIB_GETC=0; AC_SUBST([GNULIB_GETC]) GNULIB_GETCHAR=0; AC_SUBST([GNULIB_GETCHAR]) GNULIB_GETDELIM=0; AC_SUBST([GNULIB_GETDELIM]) GNULIB_GETLINE=0; AC_SUBST([GNULIB_GETLINE]) GNULIB_OBSTACK_PRINTF=0; AC_SUBST([GNULIB_OBSTACK_PRINTF]) GNULIB_OBSTACK_PRINTF_POSIX=0; AC_SUBST([GNULIB_OBSTACK_PRINTF_POSIX]) GNULIB_PCLOSE=0; AC_SUBST([GNULIB_PCLOSE]) GNULIB_PERROR=0; AC_SUBST([GNULIB_PERROR]) GNULIB_POPEN=0; AC_SUBST([GNULIB_POPEN]) GNULIB_PRINTF=0; AC_SUBST([GNULIB_PRINTF]) GNULIB_PRINTF_POSIX=0; AC_SUBST([GNULIB_PRINTF_POSIX]) GNULIB_PUTC=0; AC_SUBST([GNULIB_PUTC]) GNULIB_PUTCHAR=0; AC_SUBST([GNULIB_PUTCHAR]) GNULIB_PUTS=0; AC_SUBST([GNULIB_PUTS]) GNULIB_REMOVE=0; AC_SUBST([GNULIB_REMOVE]) GNULIB_RENAME=0; AC_SUBST([GNULIB_RENAME]) GNULIB_RENAMEAT=0; AC_SUBST([GNULIB_RENAMEAT]) GNULIB_SCANF=0; AC_SUBST([GNULIB_SCANF]) GNULIB_SNPRINTF=0; AC_SUBST([GNULIB_SNPRINTF]) GNULIB_SPRINTF_POSIX=0; AC_SUBST([GNULIB_SPRINTF_POSIX]) GNULIB_STDIO_H_NONBLOCKING=0; AC_SUBST([GNULIB_STDIO_H_NONBLOCKING]) GNULIB_STDIO_H_SIGPIPE=0; AC_SUBST([GNULIB_STDIO_H_SIGPIPE]) GNULIB_TMPFILE=0; AC_SUBST([GNULIB_TMPFILE]) GNULIB_VASPRINTF=0; AC_SUBST([GNULIB_VASPRINTF]) GNULIB_VFSCANF=0; AC_SUBST([GNULIB_VFSCANF]) GNULIB_VSCANF=0; AC_SUBST([GNULIB_VSCANF]) GNULIB_VDPRINTF=0; AC_SUBST([GNULIB_VDPRINTF]) GNULIB_VFPRINTF=0; AC_SUBST([GNULIB_VFPRINTF]) GNULIB_VFPRINTF_POSIX=0; AC_SUBST([GNULIB_VFPRINTF_POSIX]) GNULIB_VPRINTF=0; AC_SUBST([GNULIB_VPRINTF]) GNULIB_VPRINTF_POSIX=0; AC_SUBST([GNULIB_VPRINTF_POSIX]) GNULIB_VSNPRINTF=0; AC_SUBST([GNULIB_VSNPRINTF]) GNULIB_VSPRINTF_POSIX=0; AC_SUBST([GNULIB_VSPRINTF_POSIX]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_FPURGE=1; AC_SUBST([HAVE_DECL_FPURGE]) HAVE_DECL_FSEEKO=1; AC_SUBST([HAVE_DECL_FSEEKO]) HAVE_DECL_FTELLO=1; AC_SUBST([HAVE_DECL_FTELLO]) HAVE_DECL_GETDELIM=1; AC_SUBST([HAVE_DECL_GETDELIM]) HAVE_DECL_GETLINE=1; AC_SUBST([HAVE_DECL_GETLINE]) HAVE_DECL_OBSTACK_PRINTF=1; AC_SUBST([HAVE_DECL_OBSTACK_PRINTF]) HAVE_DECL_SNPRINTF=1; AC_SUBST([HAVE_DECL_SNPRINTF]) HAVE_DECL_VSNPRINTF=1; AC_SUBST([HAVE_DECL_VSNPRINTF]) HAVE_DPRINTF=1; AC_SUBST([HAVE_DPRINTF]) HAVE_FSEEKO=1; AC_SUBST([HAVE_FSEEKO]) HAVE_FTELLO=1; AC_SUBST([HAVE_FTELLO]) HAVE_PCLOSE=1; AC_SUBST([HAVE_PCLOSE]) HAVE_POPEN=1; AC_SUBST([HAVE_POPEN]) HAVE_RENAMEAT=1; AC_SUBST([HAVE_RENAMEAT]) HAVE_VASPRINTF=1; AC_SUBST([HAVE_VASPRINTF]) HAVE_VDPRINTF=1; AC_SUBST([HAVE_VDPRINTF]) REPLACE_DPRINTF=0; AC_SUBST([REPLACE_DPRINTF]) REPLACE_FCLOSE=0; AC_SUBST([REPLACE_FCLOSE]) REPLACE_FDOPEN=0; AC_SUBST([REPLACE_FDOPEN]) REPLACE_FFLUSH=0; AC_SUBST([REPLACE_FFLUSH]) REPLACE_FOPEN=0; AC_SUBST([REPLACE_FOPEN]) REPLACE_FPRINTF=0; AC_SUBST([REPLACE_FPRINTF]) REPLACE_FPURGE=0; AC_SUBST([REPLACE_FPURGE]) REPLACE_FREOPEN=0; AC_SUBST([REPLACE_FREOPEN]) REPLACE_FSEEK=0; AC_SUBST([REPLACE_FSEEK]) REPLACE_FSEEKO=0; AC_SUBST([REPLACE_FSEEKO]) REPLACE_FTELL=0; AC_SUBST([REPLACE_FTELL]) REPLACE_FTELLO=0; AC_SUBST([REPLACE_FTELLO]) REPLACE_GETDELIM=0; AC_SUBST([REPLACE_GETDELIM]) REPLACE_GETLINE=0; AC_SUBST([REPLACE_GETLINE]) REPLACE_OBSTACK_PRINTF=0; AC_SUBST([REPLACE_OBSTACK_PRINTF]) REPLACE_PERROR=0; AC_SUBST([REPLACE_PERROR]) REPLACE_POPEN=0; AC_SUBST([REPLACE_POPEN]) REPLACE_PRINTF=0; AC_SUBST([REPLACE_PRINTF]) REPLACE_REMOVE=0; AC_SUBST([REPLACE_REMOVE]) REPLACE_RENAME=0; AC_SUBST([REPLACE_RENAME]) REPLACE_RENAMEAT=0; AC_SUBST([REPLACE_RENAMEAT]) REPLACE_SNPRINTF=0; AC_SUBST([REPLACE_SNPRINTF]) REPLACE_SPRINTF=0; AC_SUBST([REPLACE_SPRINTF]) REPLACE_STDIO_READ_FUNCS=0; AC_SUBST([REPLACE_STDIO_READ_FUNCS]) REPLACE_STDIO_WRITE_FUNCS=0; AC_SUBST([REPLACE_STDIO_WRITE_FUNCS]) REPLACE_TMPFILE=0; AC_SUBST([REPLACE_TMPFILE]) REPLACE_VASPRINTF=0; AC_SUBST([REPLACE_VASPRINTF]) REPLACE_VDPRINTF=0; AC_SUBST([REPLACE_VDPRINTF]) REPLACE_VFPRINTF=0; AC_SUBST([REPLACE_VFPRINTF]) REPLACE_VPRINTF=0; AC_SUBST([REPLACE_VPRINTF]) REPLACE_VSNPRINTF=0; AC_SUBST([REPLACE_VSNPRINTF]) REPLACE_VSPRINTF=0; AC_SUBST([REPLACE_VSPRINTF]) ]) gnuastro-0.5/bootstrapped/m4/stdint_h.m40000644000175000017500000000174313217200022015237 00000000000000# stdint_h.m4 serial 9 dnl Copyright (C) 1997-2004, 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # Define HAVE_STDINT_H_WITH_UINTMAX if exists, # doesn't clash with , and declares uintmax_t. AC_DEFUN([gl_AC_HEADER_STDINT_H], [ AC_CACHE_CHECK([for stdint.h], [gl_cv_header_stdint_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[uintmax_t i = (uintmax_t) -1; return !i;]])], [gl_cv_header_stdint_h=yes], [gl_cv_header_stdint_h=no])]) if test $gl_cv_header_stdint_h = yes; then AC_DEFINE_UNQUOTED([HAVE_STDINT_H_WITH_UINTMAX], [1], [Define if exists, doesn't clash with , and declares uintmax_t. ]) fi ]) gnuastro-0.5/bootstrapped/m4/stdint.m40000644000175000017500000004373513217200022014737 00000000000000# stdint.m4 serial 51 dnl Copyright (C) 2001-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert and Bruno Haible. dnl Test whether is supported or must be substituted. AC_DEFUN_ONCE([gl_STDINT_H], [ AC_PREREQ([2.59])dnl AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_LIMITS_H]) AC_REQUIRE([gt_TYPE_WINT_T]) dnl Check for long long int and unsigned long long int. AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) if test $ac_cv_type_long_long_int = yes; then HAVE_LONG_LONG_INT=1 else HAVE_LONG_LONG_INT=0 fi AC_SUBST([HAVE_LONG_LONG_INT]) AC_REQUIRE([AC_TYPE_UNSIGNED_LONG_LONG_INT]) if test $ac_cv_type_unsigned_long_long_int = yes; then HAVE_UNSIGNED_LONG_LONG_INT=1 else HAVE_UNSIGNED_LONG_LONG_INT=0 fi AC_SUBST([HAVE_UNSIGNED_LONG_LONG_INT]) dnl Check for , in the same way as gl_WCHAR_H does. AC_CHECK_HEADERS_ONCE([wchar.h]) if test $ac_cv_header_wchar_h = yes; then HAVE_WCHAR_H=1 else HAVE_WCHAR_H=0 fi AC_SUBST([HAVE_WCHAR_H]) dnl Check for . dnl AC_INCLUDES_DEFAULT defines $ac_cv_header_inttypes_h. if test $ac_cv_header_inttypes_h = yes; then HAVE_INTTYPES_H=1 else HAVE_INTTYPES_H=0 fi AC_SUBST([HAVE_INTTYPES_H]) dnl Check for . dnl AC_INCLUDES_DEFAULT defines $ac_cv_header_sys_types_h. if test $ac_cv_header_sys_types_h = yes; then HAVE_SYS_TYPES_H=1 else HAVE_SYS_TYPES_H=0 fi AC_SUBST([HAVE_SYS_TYPES_H]) gl_CHECK_NEXT_HEADERS([stdint.h]) if test $ac_cv_header_stdint_h = yes; then HAVE_STDINT_H=1 else HAVE_STDINT_H=0 fi AC_SUBST([HAVE_STDINT_H]) dnl Now see whether we need a substitute . if test $ac_cv_header_stdint_h = yes; then AC_CACHE_CHECK([whether stdint.h conforms to C99], [gl_cv_header_working_stdint_h], [gl_cv_header_working_stdint_h=no AC_COMPILE_IFELSE([ AC_LANG_PROGRAM([[ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include /* Dragonfly defines WCHAR_MIN, WCHAR_MAX only in . */ #if !(defined WCHAR_MIN && defined WCHAR_MAX) #error "WCHAR_MIN, WCHAR_MAX not defined in " #endif ] gl_STDINT_INCLUDES [ #ifdef INT8_MAX int8_t a1 = INT8_MAX; int8_t a1min = INT8_MIN; #endif #ifdef INT16_MAX int16_t a2 = INT16_MAX; int16_t a2min = INT16_MIN; #endif #ifdef INT32_MAX int32_t a3 = INT32_MAX; int32_t a3min = INT32_MIN; #endif #ifdef INT64_MAX int64_t a4 = INT64_MAX; int64_t a4min = INT64_MIN; #endif #ifdef UINT8_MAX uint8_t b1 = UINT8_MAX; #else typedef int b1[(unsigned char) -1 != 255 ? 1 : -1]; #endif #ifdef UINT16_MAX uint16_t b2 = UINT16_MAX; #endif #ifdef UINT32_MAX uint32_t b3 = UINT32_MAX; #endif #ifdef UINT64_MAX uint64_t b4 = UINT64_MAX; #endif int_least8_t c1 = INT8_C (0x7f); int_least8_t c1max = INT_LEAST8_MAX; int_least8_t c1min = INT_LEAST8_MIN; int_least16_t c2 = INT16_C (0x7fff); int_least16_t c2max = INT_LEAST16_MAX; int_least16_t c2min = INT_LEAST16_MIN; int_least32_t c3 = INT32_C (0x7fffffff); int_least32_t c3max = INT_LEAST32_MAX; int_least32_t c3min = INT_LEAST32_MIN; int_least64_t c4 = INT64_C (0x7fffffffffffffff); int_least64_t c4max = INT_LEAST64_MAX; int_least64_t c4min = INT_LEAST64_MIN; uint_least8_t d1 = UINT8_C (0xff); uint_least8_t d1max = UINT_LEAST8_MAX; uint_least16_t d2 = UINT16_C (0xffff); uint_least16_t d2max = UINT_LEAST16_MAX; uint_least32_t d3 = UINT32_C (0xffffffff); uint_least32_t d3max = UINT_LEAST32_MAX; uint_least64_t d4 = UINT64_C (0xffffffffffffffff); uint_least64_t d4max = UINT_LEAST64_MAX; int_fast8_t e1 = INT_FAST8_MAX; int_fast8_t e1min = INT_FAST8_MIN; int_fast16_t e2 = INT_FAST16_MAX; int_fast16_t e2min = INT_FAST16_MIN; int_fast32_t e3 = INT_FAST32_MAX; int_fast32_t e3min = INT_FAST32_MIN; int_fast64_t e4 = INT_FAST64_MAX; int_fast64_t e4min = INT_FAST64_MIN; uint_fast8_t f1 = UINT_FAST8_MAX; uint_fast16_t f2 = UINT_FAST16_MAX; uint_fast32_t f3 = UINT_FAST32_MAX; uint_fast64_t f4 = UINT_FAST64_MAX; #ifdef INTPTR_MAX intptr_t g = INTPTR_MAX; intptr_t gmin = INTPTR_MIN; #endif #ifdef UINTPTR_MAX uintptr_t h = UINTPTR_MAX; #endif intmax_t i = INTMAX_MAX; uintmax_t j = UINTMAX_MAX; /* Check that SIZE_MAX has the correct type, if possible. */ #if 201112 <= __STDC_VERSION__ int k = _Generic (SIZE_MAX, size_t: 0); #elif (2 <= __GNUC__ || defined __IBM__TYPEOF__ \ || (0x5110 <= __SUNPRO_C && !__STDC__)) extern size_t k; extern __typeof__ (SIZE_MAX) k; #endif #include /* for CHAR_BIT */ #define TYPE_MINIMUM(t) \ ((t) ((t) 0 < (t) -1 ? (t) 0 : ~ TYPE_MAXIMUM (t))) #define TYPE_MAXIMUM(t) \ ((t) ((t) 0 < (t) -1 \ ? (t) -1 \ : ((((t) 1 << (sizeof (t) * CHAR_BIT - 2)) - 1) * 2 + 1))) struct s { int check_PTRDIFF: PTRDIFF_MIN == TYPE_MINIMUM (ptrdiff_t) && PTRDIFF_MAX == TYPE_MAXIMUM (ptrdiff_t) ? 1 : -1; /* Detect bug in FreeBSD 6.0 / ia64. */ int check_SIG_ATOMIC: SIG_ATOMIC_MIN == TYPE_MINIMUM (sig_atomic_t) && SIG_ATOMIC_MAX == TYPE_MAXIMUM (sig_atomic_t) ? 1 : -1; int check_SIZE: SIZE_MAX == TYPE_MAXIMUM (size_t) ? 1 : -1; int check_WCHAR: WCHAR_MIN == TYPE_MINIMUM (wchar_t) && WCHAR_MAX == TYPE_MAXIMUM (wchar_t) ? 1 : -1; /* Detect bug in mingw. */ int check_WINT: WINT_MIN == TYPE_MINIMUM (wint_t) && WINT_MAX == TYPE_MAXIMUM (wint_t) ? 1 : -1; /* Detect bugs in glibc 2.4 and Solaris 10 stdint.h, among others. */ int check_UINT8_C: (-1 < UINT8_C (0)) == (-1 < (uint_least8_t) 0) ? 1 : -1; int check_UINT16_C: (-1 < UINT16_C (0)) == (-1 < (uint_least16_t) 0) ? 1 : -1; /* Detect bugs in OpenBSD 3.9 stdint.h. */ #ifdef UINT8_MAX int check_uint8: (uint8_t) -1 == UINT8_MAX ? 1 : -1; #endif #ifdef UINT16_MAX int check_uint16: (uint16_t) -1 == UINT16_MAX ? 1 : -1; #endif #ifdef UINT32_MAX int check_uint32: (uint32_t) -1 == UINT32_MAX ? 1 : -1; #endif #ifdef UINT64_MAX int check_uint64: (uint64_t) -1 == UINT64_MAX ? 1 : -1; #endif int check_uint_least8: (uint_least8_t) -1 == UINT_LEAST8_MAX ? 1 : -1; int check_uint_least16: (uint_least16_t) -1 == UINT_LEAST16_MAX ? 1 : -1; int check_uint_least32: (uint_least32_t) -1 == UINT_LEAST32_MAX ? 1 : -1; int check_uint_least64: (uint_least64_t) -1 == UINT_LEAST64_MAX ? 1 : -1; int check_uint_fast8: (uint_fast8_t) -1 == UINT_FAST8_MAX ? 1 : -1; int check_uint_fast16: (uint_fast16_t) -1 == UINT_FAST16_MAX ? 1 : -1; int check_uint_fast32: (uint_fast32_t) -1 == UINT_FAST32_MAX ? 1 : -1; int check_uint_fast64: (uint_fast64_t) -1 == UINT_FAST64_MAX ? 1 : -1; int check_uintptr: (uintptr_t) -1 == UINTPTR_MAX ? 1 : -1; int check_uintmax: (uintmax_t) -1 == UINTMAX_MAX ? 1 : -1; int check_size: (size_t) -1 == SIZE_MAX ? 1 : -1; }; ]])], [dnl Determine whether the various *_MIN, *_MAX macros are usable dnl in preprocessor expression. We could do it by compiling a test dnl program for each of these macros. It is faster to run a program dnl that inspects the macro expansion. dnl This detects a bug on HP-UX 11.23/ia64. AC_RUN_IFELSE([ AC_LANG_PROGRAM([[ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #define __STDC_CONSTANT_MACROS 1 #define __STDC_LIMIT_MACROS 1 #include ] gl_STDINT_INCLUDES [ #include #include #define MVAL(macro) MVAL1(macro) #define MVAL1(expression) #expression static const char *macro_values[] = { #ifdef INT8_MAX MVAL (INT8_MAX), #endif #ifdef INT16_MAX MVAL (INT16_MAX), #endif #ifdef INT32_MAX MVAL (INT32_MAX), #endif #ifdef INT64_MAX MVAL (INT64_MAX), #endif #ifdef UINT8_MAX MVAL (UINT8_MAX), #endif #ifdef UINT16_MAX MVAL (UINT16_MAX), #endif #ifdef UINT32_MAX MVAL (UINT32_MAX), #endif #ifdef UINT64_MAX MVAL (UINT64_MAX), #endif NULL }; ]], [[ const char **mv; for (mv = macro_values; *mv != NULL; mv++) { const char *value = *mv; /* Test whether it looks like a cast expression. */ if (strncmp (value, "((unsigned int)"/*)*/, 15) == 0 || strncmp (value, "((unsigned short)"/*)*/, 17) == 0 || strncmp (value, "((unsigned char)"/*)*/, 16) == 0 || strncmp (value, "((int)"/*)*/, 6) == 0 || strncmp (value, "((signed short)"/*)*/, 15) == 0 || strncmp (value, "((signed char)"/*)*/, 14) == 0) return mv - macro_values + 1; } return 0; ]])], [gl_cv_header_working_stdint_h=yes], [], [case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_header_working_stdint_h="guessing yes" ;; # In general, assume it works. *) gl_cv_header_working_stdint_h="guessing yes" ;; esac ]) ]) ]) fi HAVE_C99_STDINT_H=0 HAVE_SYS_BITYPES_H=0 HAVE_SYS_INTTYPES_H=0 STDINT_H=stdint.h case "$gl_cv_header_working_stdint_h" in *yes) HAVE_C99_STDINT_H=1 dnl Now see whether the system works without dnl __STDC_CONSTANT_MACROS/__STDC_LIMIT_MACROS defined. AC_CACHE_CHECK([whether stdint.h predates C++11], [gl_cv_header_stdint_predates_cxx11_h], [gl_cv_header_stdint_predates_cxx11_h=yes AC_COMPILE_IFELSE([ AC_LANG_PROGRAM([[ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 /* work if build isn't clean */ #include ] gl_STDINT_INCLUDES [ intmax_t im = INTMAX_MAX; int32_t i32 = INT32_C (0x7fffffff); ]])], [gl_cv_header_stdint_predates_cxx11_h=no])]) if test "$gl_cv_header_stdint_predates_cxx11_h" = yes; then AC_DEFINE([__STDC_CONSTANT_MACROS], [1], [Define to 1 if the system predates C++11.]) AC_DEFINE([__STDC_LIMIT_MACROS], [1], [Define to 1 if the system predates C++11.]) fi AC_CACHE_CHECK([whether stdint.h has UINTMAX_WIDTH etc.], [gl_cv_header_stdint_width], [gl_cv_header_stdint_width=no AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H 1 #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include ]gl_STDINT_INCLUDES[ int iw = UINTMAX_WIDTH; ]])], [gl_cv_header_stdint_width=yes])]) if test "$gl_cv_header_stdint_width" = yes; then STDINT_H= fi ;; *) dnl Check for , and for dnl (used in Linux libc4 >= 4.6.7 and libc5). AC_CHECK_HEADERS([sys/inttypes.h sys/bitypes.h]) if test $ac_cv_header_sys_inttypes_h = yes; then HAVE_SYS_INTTYPES_H=1 fi if test $ac_cv_header_sys_bitypes_h = yes; then HAVE_SYS_BITYPES_H=1 fi gl_STDINT_TYPE_PROPERTIES ;; esac dnl The substitute stdint.h needs the substitute limit.h's _GL_INTEGER_WIDTH. LIMITS_H=limits.h AM_CONDITIONAL([GL_GENERATE_LIMITS_H], [test -n "$LIMITS_H"]) AC_SUBST([HAVE_C99_STDINT_H]) AC_SUBST([HAVE_SYS_BITYPES_H]) AC_SUBST([HAVE_SYS_INTTYPES_H]) AC_SUBST([STDINT_H]) AM_CONDITIONAL([GL_GENERATE_STDINT_H], [test -n "$STDINT_H"]) ]) dnl gl_STDINT_BITSIZEOF(TYPES, INCLUDES) dnl Determine the size of each of the given types in bits. AC_DEFUN([gl_STDINT_BITSIZEOF], [ dnl Use a shell loop, to avoid bloating configure, and dnl - extra AH_TEMPLATE calls, so that autoheader knows what to put into dnl config.h.in, dnl - extra AC_SUBST calls, so that the right substitutions are made. m4_foreach_w([gltype], [$1], [AH_TEMPLATE([BITSIZEOF_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]), [Define to the number of bits in type ']gltype['.])]) for gltype in $1 ; do AC_CACHE_CHECK([for bit size of $gltype], [gl_cv_bitsizeof_${gltype}], [AC_COMPUTE_INT([result], [sizeof ($gltype) * CHAR_BIT], [$2 #include ], [result=unknown]) eval gl_cv_bitsizeof_${gltype}=\$result ]) eval result=\$gl_cv_bitsizeof_${gltype} if test $result = unknown; then dnl Use a nonempty default, because some compilers, such as IRIX 5 cc, dnl do a syntax check even on unused #if conditions and give an error dnl on valid C code like this: dnl #if 0 dnl # if > 32 dnl # endif dnl #endif result=0 fi GLTYPE=`echo "$gltype" | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` AC_DEFINE_UNQUOTED([BITSIZEOF_${GLTYPE}], [$result]) eval BITSIZEOF_${GLTYPE}=\$result done m4_foreach_w([gltype], [$1], [AC_SUBST([BITSIZEOF_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]))]) ]) dnl gl_CHECK_TYPES_SIGNED(TYPES, INCLUDES) dnl Determine the signedness of each of the given types. dnl Define HAVE_SIGNED_TYPE if type is signed. AC_DEFUN([gl_CHECK_TYPES_SIGNED], [ dnl Use a shell loop, to avoid bloating configure, and dnl - extra AH_TEMPLATE calls, so that autoheader knows what to put into dnl config.h.in, dnl - extra AC_SUBST calls, so that the right substitutions are made. m4_foreach_w([gltype], [$1], [AH_TEMPLATE([HAVE_SIGNED_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]), [Define to 1 if ']gltype[' is a signed integer type.])]) for gltype in $1 ; do AC_CACHE_CHECK([whether $gltype is signed], [gl_cv_type_${gltype}_signed], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([$2[ int verify[2 * (($gltype) -1 < ($gltype) 0) - 1];]])], result=yes, result=no) eval gl_cv_type_${gltype}_signed=\$result ]) eval result=\$gl_cv_type_${gltype}_signed GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` if test "$result" = yes; then AC_DEFINE_UNQUOTED([HAVE_SIGNED_${GLTYPE}], [1]) eval HAVE_SIGNED_${GLTYPE}=1 else eval HAVE_SIGNED_${GLTYPE}=0 fi done m4_foreach_w([gltype], [$1], [AC_SUBST([HAVE_SIGNED_]m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_]))]) ]) dnl gl_INTEGER_TYPE_SUFFIX(TYPES, INCLUDES) dnl Determine the suffix to use for integer constants of the given types. dnl Define t_SUFFIX for each such type. AC_DEFUN([gl_INTEGER_TYPE_SUFFIX], [ dnl Use a shell loop, to avoid bloating configure, and dnl - extra AH_TEMPLATE calls, so that autoheader knows what to put into dnl config.h.in, dnl - extra AC_SUBST calls, so that the right substitutions are made. m4_foreach_w([gltype], [$1], [AH_TEMPLATE(m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_])[_SUFFIX], [Define to l, ll, u, ul, ull, etc., as suitable for constants of type ']gltype['.])]) for gltype in $1 ; do AC_CACHE_CHECK([for $gltype integer literal suffix], [gl_cv_type_${gltype}_suffix], [eval gl_cv_type_${gltype}_suffix=no eval result=\$gl_cv_type_${gltype}_signed if test "$result" = yes; then glsufu= else glsufu=u fi for glsuf in "$glsufu" ${glsufu}l ${glsufu}ll ${glsufu}i64; do case $glsuf in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; i64) gltype1='__int64';; u) gltype1='unsigned int';; ul) gltype1='unsigned long int';; ull) gltype1='unsigned long long int';; ui64)gltype1='unsigned __int64';; esac AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([$2[ extern $gltype foo; extern $gltype1 foo;]])], [eval gl_cv_type_${gltype}_suffix=\$glsuf]) eval result=\$gl_cv_type_${gltype}_suffix test "$result" != no && break done]) GLTYPE=`echo $gltype | tr 'abcdefghijklmnopqrstuvwxyz ' 'ABCDEFGHIJKLMNOPQRSTUVWXYZ_'` eval result=\$gl_cv_type_${gltype}_suffix test "$result" = no && result= eval ${GLTYPE}_SUFFIX=\$result AC_DEFINE_UNQUOTED([${GLTYPE}_SUFFIX], [$result]) done m4_foreach_w([gltype], [$1], [AC_SUBST(m4_translit(gltype,[abcdefghijklmnopqrstuvwxyz ],[ABCDEFGHIJKLMNOPQRSTUVWXYZ_])[_SUFFIX])]) ]) dnl gl_STDINT_INCLUDES AC_DEFUN([gl_STDINT_INCLUDES], [[ /* BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #if HAVE_WCHAR_H # include # include # include #endif ]]) dnl gl_STDINT_TYPE_PROPERTIES dnl Compute HAVE_SIGNED_t, BITSIZEOF_t and t_SUFFIX, for all the types t dnl of interest to stdint.in.h. AC_DEFUN([gl_STDINT_TYPE_PROPERTIES], [ AC_REQUIRE([gl_MULTIARCH]) if test $APPLE_UNIVERSAL_BUILD = 0; then gl_STDINT_BITSIZEOF([ptrdiff_t size_t], [gl_STDINT_INCLUDES]) fi gl_STDINT_BITSIZEOF([sig_atomic_t wchar_t wint_t], [gl_STDINT_INCLUDES]) gl_CHECK_TYPES_SIGNED([sig_atomic_t wchar_t wint_t], [gl_STDINT_INCLUDES]) gl_cv_type_ptrdiff_t_signed=yes gl_cv_type_size_t_signed=no if test $APPLE_UNIVERSAL_BUILD = 0; then gl_INTEGER_TYPE_SUFFIX([ptrdiff_t size_t], [gl_STDINT_INCLUDES]) fi gl_INTEGER_TYPE_SUFFIX([sig_atomic_t wchar_t wint_t], [gl_STDINT_INCLUDES]) dnl If wint_t is smaller than 'int', it cannot satisfy the ISO C 99 dnl requirement that wint_t is "unchanged by default argument promotions". dnl In this case gnulib's and override wint_t. dnl Set the variable BITSIZEOF_WINT_T accordingly. if test $GNULIB_OVERRIDES_WINT_T = 1; then BITSIZEOF_WINT_T=32 fi ]) dnl Autoconf >= 2.61 has AC_COMPUTE_INT built-in. dnl Remove this when we can assume autoconf >= 2.61. m4_ifdef([AC_COMPUTE_INT], [], [ AC_DEFUN([AC_COMPUTE_INT], [_AC_COMPUTE_INT([$2],[$1],[$3],[$4])]) ]) gnuastro-0.5/bootstrapped/m4/stddef_h.m40000644000175000017500000000321613217200022015200 00000000000000dnl A placeholder for , for platforms that have issues. # stddef_h.m4 serial 5 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_STDDEF_H], [ AC_REQUIRE([gl_STDDEF_H_DEFAULTS]) AC_REQUIRE([gt_TYPE_WCHAR_T]) STDDEF_H= AC_CHECK_TYPE([max_align_t], [], [HAVE_MAX_ALIGN_T=0; STDDEF_H=stddef.h], [[#include ]]) if test $gt_cv_c_wchar_t = no; then HAVE_WCHAR_T=0 STDDEF_H=stddef.h fi AC_CACHE_CHECK([whether NULL can be used in arbitrary expressions], [gl_cv_decl_null_works], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include int test[2 * (sizeof NULL == sizeof (void *)) -1]; ]])], [gl_cv_decl_null_works=yes], [gl_cv_decl_null_works=no])]) if test $gl_cv_decl_null_works = no; then REPLACE_NULL=1 STDDEF_H=stddef.h fi AC_SUBST([STDDEF_H]) AM_CONDITIONAL([GL_GENERATE_STDDEF_H], [test -n "$STDDEF_H"]) if test -n "$STDDEF_H"; then gl_NEXT_HEADERS([stddef.h]) fi ]) AC_DEFUN([gl_STDDEF_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_STDDEF_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_STDDEF_H_DEFAULTS], [ dnl Assume proper GNU behavior unless another module says otherwise. REPLACE_NULL=0; AC_SUBST([REPLACE_NULL]) HAVE_MAX_ALIGN_T=1; AC_SUBST([HAVE_MAX_ALIGN_T]) HAVE_WCHAR_T=1; AC_SUBST([HAVE_WCHAR_T]) ]) gnuastro-0.5/bootstrapped/m4/stdbool.m40000644000175000017500000000671613217200022015076 00000000000000# Check for stdbool.h that conforms to C99. dnl Copyright (C) 2002-2006, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. #serial 7 # Prepare for substituting if it is not supported. AC_DEFUN([AM_STDBOOL_H], [ AC_REQUIRE([AC_CHECK_HEADER_STDBOOL]) # Define two additional variables used in the Makefile substitution. if test "$ac_cv_header_stdbool_h" = yes; then STDBOOL_H='' else STDBOOL_H='stdbool.h' fi AC_SUBST([STDBOOL_H]) AM_CONDITIONAL([GL_GENERATE_STDBOOL_H], [test -n "$STDBOOL_H"]) if test "$ac_cv_type__Bool" = yes; then HAVE__BOOL=1 else HAVE__BOOL=0 fi AC_SUBST([HAVE__BOOL]) ]) # AM_STDBOOL_H will be renamed to gl_STDBOOL_H in the future. AC_DEFUN([gl_STDBOOL_H], [AM_STDBOOL_H]) # This version of the macro is needed in autoconf <= 2.68. AC_DEFUN([AC_CHECK_HEADER_STDBOOL], [AC_CACHE_CHECK([for stdbool.h that conforms to C99], [ac_cv_header_stdbool_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #ifdef __cplusplus typedef bool Bool; #else typedef _Bool Bool; #ifndef bool "error: bool is not defined" #endif #ifndef false "error: false is not defined" #endif #if false "error: false is not 0" #endif #ifndef true "error: true is not defined" #endif #if true != 1 "error: true is not 1" #endif #endif #ifndef __bool_true_false_are_defined "error: __bool_true_false_are_defined is not defined" #endif struct s { Bool s: 1; Bool t; bool u: 1; bool v; } s; char a[true == 1 ? 1 : -1]; char b[false == 0 ? 1 : -1]; char c[__bool_true_false_are_defined == 1 ? 1 : -1]; char d[(bool) 0.5 == true ? 1 : -1]; /* See body of main program for 'e'. */ char f[(Bool) 0.0 == false ? 1 : -1]; char g[true]; char h[sizeof (Bool)]; char i[sizeof s.t]; enum { j = false, k = true, l = false * true, m = true * 256 }; /* The following fails for HP aC++/ANSI C B3910B A.05.55 [Dec 04 2003]. */ Bool n[m]; char o[sizeof n == m * sizeof n[0] ? 1 : -1]; char p[-1 - (Bool) 0 < 0 && -1 - (bool) 0 < 0 ? 1 : -1]; /* Catch a bug in an HP-UX C compiler. See https://gcc.gnu.org/ml/gcc-patches/2003-12/msg02303.html https://lists.gnu.org/r/bug-coreutils/2005-11/msg00161.html */ Bool q = true; Bool *pq = &q; bool *qq = &q; ]], [[ bool e = &s; *pq |= q; *pq |= ! q; *qq |= q; *qq |= ! q; /* Refer to every declared value, to avoid compiler optimizations. */ return (!a + !b + !c + !d + !e + !f + !g + !h + !i + !!j + !k + !!l + !m + !n + !o + !p + !q + !pq + !qq); ]])], [ac_cv_header_stdbool_h=yes], [ac_cv_header_stdbool_h=no])]) AC_CHECK_TYPES([_Bool]) ]) gnuastro-0.5/bootstrapped/m4/stdalign.m40000644000175000017500000000442713217200022015232 00000000000000# Check for stdalign.h that conforms to C11. dnl Copyright 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Prepare for substituting if it is not supported. AC_DEFUN([gl_STDALIGN_H], [ AC_CACHE_CHECK([for working stdalign.h], [gl_cv_header_working_stdalign_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include /* Test that alignof yields a result consistent with offsetof. This catches GCC bug 52023 . */ #ifdef __cplusplus template struct alignof_helper { char a; t b; }; # define ao(type) offsetof (alignof_helper, b) #else # define ao(type) offsetof (struct { char a; type b; }, b) #endif char test_double[ao (double) % _Alignof (double) == 0 ? 1 : -1]; char test_long[ao (long int) % _Alignof (long int) == 0 ? 1 : -1]; char test_alignof[alignof (double) == _Alignof (double) ? 1 : -1]; /* Test _Alignas only on platforms where gnulib can help. */ #if \ ((defined __cplusplus && 201103 <= __cplusplus) \ || (defined __APPLE__ && defined __MACH__ \ ? 4 < __GNUC__ + (1 <= __GNUC_MINOR__) \ : __GNUC__) \ || (__ia64 && (61200 <= __HP_cc || 61200 <= __HP_aCC)) \ || __ICC || 0x590 <= __SUNPRO_C || 0x0600 <= __xlC__ \ || 1300 <= _MSC_VER) struct alignas_test { char c; char alignas (8) alignas_8; }; char test_alignas[offsetof (struct alignas_test, alignas_8) == 8 ? 1 : -1]; #endif ]])], [gl_cv_header_working_stdalign_h=yes], [gl_cv_header_working_stdalign_h=no])]) if test $gl_cv_header_working_stdalign_h = yes; then STDALIGN_H='' else STDALIGN_H='stdalign.h' fi AC_SUBST([STDALIGN_H]) AM_CONDITIONAL([GL_GENERATE_STDALIGN_H], [test -n "$STDALIGN_H"]) ]) gnuastro-0.5/bootstrapped/m4/stat.m40000644000175000017500000000461713217200022014401 00000000000000# serial 13 # Copyright (C) 2009-2017 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_STAT], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([lstat]) case "$host_os" in mingw*) dnl On this platform, the original stat() returns st_atime, st_mtime, dnl st_ctime values that are affected by the time zone. REPLACE_STAT=1 ;; *) dnl AIX 7.1, Solaris 9, mingw64 mistakenly succeed on stat("file/"). dnl (For mingw, this is due to a broken stat() override in libmingwex.a.) dnl FreeBSD 7.2 mistakenly succeeds on stat("link-to-file/"). AC_CACHE_CHECK([whether stat handles trailing slashes on files], [gl_cv_func_stat_file_slash], [touch conftest.tmp # Assume that if we have lstat, we can also check symlinks. if test $ac_cv_func_lstat = yes; then ln -s conftest.tmp conftest.lnk fi AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[int result = 0; struct stat st; if (!stat ("conftest.tmp/", &st)) result |= 1; #if HAVE_LSTAT if (!stat ("conftest.lnk/", &st)) result |= 2; #endif return result; ]])], [gl_cv_func_stat_file_slash=yes], [gl_cv_func_stat_file_slash=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_stat_file_slash="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_stat_file_slash="guessing no" ;; esac ]) rm -f conftest.tmp conftest.lnk]) case $gl_cv_func_stat_file_slash in *no) REPLACE_STAT=1 AC_DEFINE([REPLACE_FUNC_STAT_FILE], [1], [Define to 1 if stat needs help when passed a file name with a trailing slash]);; esac case $host_os in dnl Solaris stat can return a negative tv_nsec. solaris*) REPLACE_FSTAT=1 ;; esac ;; esac ]) # Prerequisites of lib/stat.c and lib/stat-w32.c. AC_DEFUN([gl_PREREQ_STAT], [ AC_REQUIRE([gl_HEADER_SYS_STAT_H]) : ]) gnuastro-0.5/bootstrapped/m4/stat-time.m40000644000175000017500000000605713217200022015335 00000000000000# Checks for stat-related time functions. # Copyright (C) 1998-1999, 2001, 2003, 2005-2007, 2009-2017 Free Software # Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # st_atim.tv_nsec - Linux, Solaris, Cygwin # st_atimespec.tv_nsec - FreeBSD, NetBSD, if ! defined _POSIX_SOURCE # st_atimensec - FreeBSD, NetBSD, if defined _POSIX_SOURCE # st_atim.st__tim.tv_nsec - UnixWare (at least 2.1.2 through 7.1) # st_birthtimespec - FreeBSD, NetBSD (hidden on OpenBSD 3.9, anyway) # st_birthtim - Cygwin 1.7.0+ AC_DEFUN([gl_STAT_TIME], [ AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS_ONCE([sys/time.h]) AC_CHECK_MEMBERS([struct stat.st_atim.tv_nsec], [AC_CACHE_CHECK([whether struct stat.st_atim is of type struct timespec], [ac_cv_typeof_struct_stat_st_atim_is_struct_timespec], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM( [[ #include #include #if HAVE_SYS_TIME_H # include #endif #include struct timespec ts; struct stat st; ]], [[ st.st_atim = ts; ]])], [ac_cv_typeof_struct_stat_st_atim_is_struct_timespec=yes], [ac_cv_typeof_struct_stat_st_atim_is_struct_timespec=no])]) if test $ac_cv_typeof_struct_stat_st_atim_is_struct_timespec = yes; then AC_DEFINE([TYPEOF_STRUCT_STAT_ST_ATIM_IS_STRUCT_TIMESPEC], [1], [Define to 1 if the type of the st_atim member of a struct stat is struct timespec.]) fi], [AC_CHECK_MEMBERS([struct stat.st_atimespec.tv_nsec], [], [AC_CHECK_MEMBERS([struct stat.st_atimensec], [], [AC_CHECK_MEMBERS([struct stat.st_atim.st__tim.tv_nsec], [], [], [#include #include ])], [#include #include ])], [#include #include ])], [#include #include ]) ]) # Check for st_birthtime, a feature from UFS2 (FreeBSD, NetBSD, OpenBSD, etc.) # and NTFS (Cygwin). # There was a time when this field was named st_createtime (21 June # 2002 to 16 July 2002) But that window is very small and applied only # to development code, so systems still using that configuration are # not supported. See revisions 1.10 and 1.11 of FreeBSD's # src/sys/ufs/ufs/dinode.h. # AC_DEFUN([gl_STAT_BIRTHTIME], [ AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS_ONCE([sys/time.h]) AC_CHECK_MEMBERS([struct stat.st_birthtimespec.tv_nsec], [], [AC_CHECK_MEMBERS([struct stat.st_birthtimensec], [], [AC_CHECK_MEMBERS([struct stat.st_birthtim.tv_nsec], [], [], [#include #include ])], [#include #include ])], [#include #include ]) ]) gnuastro-0.5/bootstrapped/m4/ssize_t.m40000644000175000017500000000146313217200022015102 00000000000000# ssize_t.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2001-2003, 2006, 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Test whether ssize_t is defined. AC_DEFUN([gt_TYPE_SSIZE_T], [ AC_CACHE_CHECK([for ssize_t], [gt_cv_ssize_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[int x = sizeof (ssize_t *) + sizeof (ssize_t); return !x;]])], [gt_cv_ssize_t=yes], [gt_cv_ssize_t=no])]) if test $gt_cv_ssize_t = no; then AC_DEFINE([ssize_t], [int], [Define as a signed type of the same size as size_t.]) fi ]) gnuastro-0.5/bootstrapped/m4/sockpfaf.m40000644000175000017500000000522613217200022015217 00000000000000# sockpfaf.m4 serial 8 dnl Copyright (C) 2004, 2006, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Test for some common socket protocol families (PF_INET, PF_INET6, ...) dnl and some common address families (AF_INET, AF_INET6, ...). dnl This test assumes that a system supports an address family if and only if dnl it supports the corresponding protocol family. dnl From Bruno Haible. AC_DEFUN([gl_SOCKET_FAMILIES], [ AC_REQUIRE([gl_HEADER_SYS_SOCKET]) AC_CHECK_HEADERS_ONCE([netinet/in.h]) AC_MSG_CHECKING([for IPv4 sockets]) AC_CACHE_VAL([gl_cv_socket_ipv4], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_NETINET_IN_H #include #endif #ifdef HAVE_WINSOCK2_H #include #endif]], [[int x = AF_INET; struct in_addr y; struct sockaddr_in z; if (&x && &y && &z) return 0;]])], gl_cv_socket_ipv4=yes, gl_cv_socket_ipv4=no)]) AC_MSG_RESULT([$gl_cv_socket_ipv4]) if test $gl_cv_socket_ipv4 = yes; then AC_DEFINE([HAVE_IPV4], [1], [Define to 1 if defines AF_INET.]) fi AC_MSG_CHECKING([for IPv6 sockets]) AC_CACHE_VAL([gl_cv_socket_ipv6], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_NETINET_IN_H #include #endif #ifdef HAVE_WINSOCK2_H #include #endif #ifdef HAVE_WS2TCPIP_H #include #endif]], [[int x = AF_INET6; struct in6_addr y; struct sockaddr_in6 z; if (&x && &y && &z) return 0;]])], gl_cv_socket_ipv6=yes, gl_cv_socket_ipv6=no)]) AC_MSG_RESULT([$gl_cv_socket_ipv6]) if test $gl_cv_socket_ipv6 = yes; then AC_DEFINE([HAVE_IPV6], [1], [Define to 1 if defines AF_INET6.]) fi ]) AC_DEFUN([gl_SOCKET_FAMILY_UNIX], [ AC_REQUIRE([gl_HEADER_SYS_SOCKET]) AC_CHECK_HEADERS_ONCE([sys/un.h]) AC_MSG_CHECKING([for UNIX domain sockets]) AC_CACHE_VAL([gl_cv_socket_unix], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include #ifdef HAVE_SYS_SOCKET_H #include #endif #ifdef HAVE_SYS_UN_H #include #endif #ifdef HAVE_WINSOCK2_H #include #endif]], [[int x = AF_UNIX; struct sockaddr_un y; if (&x && &y) return 0;]])], gl_cv_socket_unix=yes, gl_cv_socket_unix=no)]) AC_MSG_RESULT([$gl_cv_socket_unix]) if test $gl_cv_socket_unix = yes; then AC_DEFINE([HAVE_UNIXSOCKET], [1], [Define to 1 if defines AF_UNIX.]) fi ]) gnuastro-0.5/bootstrapped/m4/socklen.m40000644000175000017500000000623613217200022015063 00000000000000# socklen.m4 serial 10 dnl Copyright (C) 2005-2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Albert Chin, Windows fixes from Simon Josefsson. dnl Check for socklen_t: historically on BSD it is an int, and in dnl POSIX 1g it is a type of its own, but some platforms use different dnl types for the argument to getsockopt, getpeername, etc.: dnl HP-UX 10.20, IRIX 6.5, OSF/1 4.0, Interix 3.5, BeOS. dnl So we have to test to find something that will work. AC_DEFUN([gl_TYPE_SOCKLEN_T], [AC_REQUIRE([gl_CHECK_SOCKET_HEADERS])dnl AC_CHECK_TYPE([socklen_t], , [AC_MSG_CHECKING([for socklen_t equivalent]) AC_CACHE_VAL([gl_cv_socklen_t_equiv], [# Systems have either "struct sockaddr *" or # "void *" as the second argument to getpeername gl_cv_socklen_t_equiv= for arg2 in "struct sockaddr" void; do for t in int size_t "unsigned int" "long int" "unsigned long int"; do AC_COMPILE_IFELSE([AC_LANG_PROGRAM( [[#include #include int getpeername (int, $arg2 *, $t *);]], [[$t len; getpeername (0, 0, &len);]])], [gl_cv_socklen_t_equiv="$t"]) test "$gl_cv_socklen_t_equiv" != "" && break done test "$gl_cv_socklen_t_equiv" != "" && break done ]) if test "$gl_cv_socklen_t_equiv" = ""; then AC_MSG_ERROR([Cannot find a type to use in place of socklen_t]) fi AC_MSG_RESULT([$gl_cv_socklen_t_equiv]) AC_DEFINE_UNQUOTED([socklen_t], [$gl_cv_socklen_t_equiv], [type to use in place of socklen_t if not defined])], [gl_SOCKET_HEADERS])]) dnl On mingw32, socklen_t is in ws2tcpip.h ('int'), so we try to find dnl it there too. But on Cygwin, wc2tcpip.h must not be included. Users dnl of this module should use the same include pattern as gl_SOCKET_HEADERS. dnl When you change this macro, keep also in sync: dnl - gl_CHECK_SOCKET_HEADERS, dnl - the Include section of modules/socklen. AC_DEFUN([gl_SOCKET_HEADERS], [ /* is not needed according to POSIX, but the in i386-unknown-freebsd4.10 and powerpc-apple-darwin5.5 required it. */ #include #if HAVE_SYS_SOCKET_H # include #elif HAVE_WS2TCPIP_H # include #endif ]) dnl Tests for the existence of the header for socket facilities. dnl Defines the C macros HAVE_SYS_SOCKET_H, HAVE_WS2TCPIP_H. dnl This macro must match gl_SOCKET_HEADERS. AC_DEFUN([gl_CHECK_SOCKET_HEADERS], [AC_CHECK_HEADERS_ONCE([sys/socket.h]) if test $ac_cv_header_sys_socket_h = no; then dnl We cannot use AC_CHECK_HEADERS_ONCE here, because that would make dnl the check for those headers unconditional; yet cygwin reports dnl that the headers are present but cannot be compiled (since on dnl cygwin, all socket information should come from sys/socket.h). AC_CHECK_HEADERS([ws2tcpip.h]) fi ]) gnuastro-0.5/bootstrapped/m4/sockets.m40000644000175000017500000000070713217200022015075 00000000000000# sockets.m4 serial 7 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_SOCKETS], [ AC_REQUIRE([AC_C_INLINE]) AC_REQUIRE([gl_SOCKETLIB]) gl_PREREQ_SOCKETS ]) # Prerequisites of lib/sockets.c. AC_DEFUN([gl_PREREQ_SOCKETS], [ : ]) gnuastro-0.5/bootstrapped/m4/socketlib.m40000644000175000017500000000524413217200022015402 00000000000000# socketlib.m4 serial 1 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl gl_SOCKETLIB dnl Determines the library to use for socket functions. dnl Sets and AC_SUBSTs LIBSOCKET. AC_DEFUN([gl_SOCKETLIB], [ gl_PREREQ_SYS_H_WINSOCK2 dnl for HAVE_WINSOCK2_H LIBSOCKET= if test $HAVE_WINSOCK2_H = 1; then dnl Native Windows API (not Cygwin). AC_CACHE_CHECK([if we need to call WSAStartup in winsock2.h and -lws2_32], [gl_cv_func_wsastartup], [ gl_save_LIBS="$LIBS" LIBS="$LIBS -lws2_32" AC_LINK_IFELSE([AC_LANG_PROGRAM([[ #ifdef HAVE_WINSOCK2_H # include #endif]], [[ WORD wVersionRequested = MAKEWORD(1, 1); WSADATA wsaData; int err = WSAStartup(wVersionRequested, &wsaData); WSACleanup ();]])], gl_cv_func_wsastartup=yes, gl_cv_func_wsastartup=no) LIBS="$gl_save_LIBS" ]) if test "$gl_cv_func_wsastartup" = "yes"; then AC_DEFINE([WINDOWS_SOCKETS], [1], [Define if WSAStartup is needed.]) LIBSOCKET='-lws2_32' fi else dnl Unix API. dnl Solaris has most socket functions in libsocket. dnl Haiku has most socket functions in libnetwork. dnl BeOS has most socket functions in libnet. AC_CACHE_CHECK([for library containing setsockopt], [gl_cv_lib_socket], [ gl_cv_lib_socket= AC_LINK_IFELSE([AC_LANG_PROGRAM([[extern #ifdef __cplusplus "C" #endif char setsockopt();]], [[setsockopt();]])], [], [gl_save_LIBS="$LIBS" LIBS="$gl_save_LIBS -lsocket" AC_LINK_IFELSE([AC_LANG_PROGRAM([[extern #ifdef __cplusplus "C" #endif char setsockopt();]], [[setsockopt();]])], [gl_cv_lib_socket="-lsocket"]) if test -z "$gl_cv_lib_socket"; then LIBS="$gl_save_LIBS -lnetwork" AC_LINK_IFELSE([AC_LANG_PROGRAM([[extern #ifdef __cplusplus "C" #endif char setsockopt();]], [[setsockopt();]])], [gl_cv_lib_socket="-lnetwork"]) if test -z "$gl_cv_lib_socket"; then LIBS="$gl_save_LIBS -lnet" AC_LINK_IFELSE([AC_LANG_PROGRAM([[extern #ifdef __cplusplus "C" #endif char setsockopt();]], [[setsockopt();]])], [gl_cv_lib_socket="-lnet"]) fi fi LIBS="$gl_save_LIBS" ]) if test -z "$gl_cv_lib_socket"; then gl_cv_lib_socket="none needed" fi ]) if test "$gl_cv_lib_socket" != "none needed"; then LIBSOCKET="$gl_cv_lib_socket" fi fi AC_SUBST([LIBSOCKET]) ]) gnuastro-0.5/bootstrapped/m4/sleep.m40000644000175000017500000000420313217200022014525 00000000000000# sleep.m4 serial 8 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SLEEP], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl We expect to see the declaration of sleep() in a header file. dnl Older versions of mingw have a sleep() function that is an alias to dnl _sleep() in MSVCRT. It has a different signature than POSIX sleep(): dnl it takes the number of milliseconds as argument and returns void. dnl mingw does not declare this function. AC_CHECK_DECLS([sleep], , , [[#include ]]) AC_CHECK_FUNCS_ONCE([sleep]) if test $ac_cv_have_decl_sleep != yes; then HAVE_SLEEP=0 else dnl Cygwin 1.5.x has a bug where sleep can't exceed 49.7 days. AC_CACHE_CHECK([for working sleep], [gl_cv_func_sleep_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include #include static void handle_alarm (int sig) { if (sig != SIGALRM) _exit (2); } ]], [[ /* Failure to compile this test due to missing alarm is okay, since all such platforms (mingw) also lack sleep. */ unsigned int pentecost = 50 * 24 * 60 * 60; /* 50 days. */ unsigned int remaining; signal (SIGALRM, handle_alarm); alarm (1); remaining = sleep (pentecost); if (remaining > pentecost) return 3; if (remaining <= pentecost - 10) return 4; return 0; ]])], [gl_cv_func_sleep_works=yes], [gl_cv_func_sleep_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_sleep_works="guessing yes" ;; # Guess no on native Windows. mingw*) gl_cv_func_sleep_works="guessing no" ;; # If we don't know, assume the worst. *) gl_cv_func_sleep_works="guessing no" ;; esac ])]) case "$gl_cv_func_sleep_works" in *yes) ;; *) REPLACE_SLEEP=1 ;; esac fi ]) gnuastro-0.5/bootstrapped/m4/size_max.m40000644000175000017500000000577013217200022015246 00000000000000# size_max.m4 serial 10 dnl Copyright (C) 2003, 2005-2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_DEFUN([gl_SIZE_MAX], [ AC_CHECK_HEADERS([stdint.h]) dnl First test whether the system already has SIZE_MAX. AC_CACHE_CHECK([for SIZE_MAX], [gl_cv_size_max], [ gl_cv_size_max= AC_EGREP_CPP([Found it], [ #include #if HAVE_STDINT_H #include #endif #ifdef SIZE_MAX Found it #endif ], [gl_cv_size_max=yes]) if test -z "$gl_cv_size_max"; then dnl Define it ourselves. Here we assume that the type 'size_t' is not wider dnl than the type 'unsigned long'. Try hard to find a definition that can dnl be used in a preprocessor #if, i.e. doesn't contain a cast. AC_COMPUTE_INT([size_t_bits_minus_1], [sizeof (size_t) * CHAR_BIT - 1], [#include #include ], [size_t_bits_minus_1=]) AC_COMPUTE_INT([fits_in_uint], [sizeof (size_t) <= sizeof (unsigned int)], [#include ], [fits_in_uint=]) if test -n "$size_t_bits_minus_1" && test -n "$fits_in_uint"; then if test $fits_in_uint = 1; then dnl Even though SIZE_MAX fits in an unsigned int, it must be of type dnl 'unsigned long' if the type 'size_t' is the same as 'unsigned long'. AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include extern size_t foo; extern unsigned long foo; ]], [[]])], [fits_in_uint=0]) fi dnl We cannot use 'expr' to simplify this expression, because 'expr' dnl works only with 'long' integers in the host environment, while we dnl might be cross-compiling from a 32-bit platform to a 64-bit platform. if test $fits_in_uint = 1; then gl_cv_size_max="(((1U << $size_t_bits_minus_1) - 1) * 2 + 1)" else gl_cv_size_max="(((1UL << $size_t_bits_minus_1) - 1) * 2 + 1)" fi else dnl Shouldn't happen, but who knows... gl_cv_size_max='((size_t)~(size_t)0)' fi fi ]) if test "$gl_cv_size_max" != yes; then AC_DEFINE_UNQUOTED([SIZE_MAX], [$gl_cv_size_max], [Define as the maximum value of type 'size_t', if the system doesn't define it.]) fi dnl Don't redefine SIZE_MAX in config.h if config.h is re-included after dnl . Remember that the #undef in AH_VERBATIM gets replaced with dnl #define by AC_DEFINE_UNQUOTED. AH_VERBATIM([SIZE_MAX], [/* Define as the maximum value of type 'size_t', if the system doesn't define it. */ #ifndef SIZE_MAX # undef SIZE_MAX #endif]) ]) dnl Autoconf >= 2.61 has AC_COMPUTE_INT built-in. dnl Remove this when we can assume autoconf >= 2.61. m4_ifdef([AC_COMPUTE_INT], [], [ AC_DEFUN([AC_COMPUTE_INT], [_AC_COMPUTE_INT([$2],[$1],[$3],[$4])]) ]) gnuastro-0.5/bootstrapped/m4/signbit.m40000644000175000017500000003014613217200022015061 00000000000000# signbit.m4 serial 15 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_SIGNBIT], [ AC_REQUIRE([gl_MATH_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([for signbit macro], [gl_cv_func_signbit], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include /* If signbit is defined as a function, don't use it, since calling it for 'float' or 'long double' arguments would involve conversions. If signbit is not declared at all but exists as a library function, don't use it, since the prototype may not match. If signbit is not declared at all but exists as a compiler built-in, don't use it, since it's preferable to use __builtin_signbit* (no warnings, no conversions). */ #ifndef signbit # error "signbit should be a macro" #endif #include ]gl_SIGNBIT_TEST_PROGRAM ])], [gl_cv_func_signbit=yes], [gl_cv_func_signbit=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_signbit="guessing yes" ;; # Guess yes on native Windows. mingw*) gl_cv_func_signbit="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_signbit="guessing no" ;; esac ]) ]) dnl GCC 4.0 and newer provides three built-ins for signbit. dnl They can be used without warnings, also in C++, regardless of . dnl But they may expand to calls to functions, which may or may not be in dnl libc. AC_CACHE_CHECK([for signbit compiler built-ins], [gl_cv_func_signbit_gcc], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #if __GNUC__ >= 4 # define signbit(x) \ (sizeof (x) == sizeof (long double) ? __builtin_signbitl (x) : \ sizeof (x) == sizeof (double) ? __builtin_signbit (x) : \ __builtin_signbitf (x)) #else # error "signbit should be three compiler built-ins" #endif #include ]gl_SIGNBIT_TEST_PROGRAM ])], [gl_cv_func_signbit_gcc=yes], [gl_cv_func_signbit_gcc=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_signbit_gcc="guessing yes" ;; # Guess yes on mingw, no on MSVC. mingw*) if test -n "$GCC"; then gl_cv_func_signbit_gcc="guessing yes" else gl_cv_func_signbit_gcc="guessing no" fi ;; # If we don't know, assume the worst. *) gl_cv_func_signbit_gcc="guessing no" ;; esac ]) ]) dnl Use the compiler built-ins whenever possible, because they are more dnl efficient than the system library functions (if they exist). case "$gl_cv_func_signbit_gcc" in *yes) REPLACE_SIGNBIT_USING_GCC=1 ;; *) case "$gl_cv_func_signbit" in *yes) ;; *) dnl REPLACE_SIGNBIT=1 makes sure the signbit[fdl] functions get built. REPLACE_SIGNBIT=1 gl_FLOAT_SIGN_LOCATION gl_DOUBLE_SIGN_LOCATION gl_LONG_DOUBLE_SIGN_LOCATION if test "$gl_cv_cc_float_signbit" = unknown; then dnl Test whether copysignf() is declared. AC_CHECK_DECLS([copysignf], , , [[#include ]]) if test "$ac_cv_have_decl_copysignf" = yes; then dnl Test whether copysignf() can be used without libm. AC_CACHE_CHECK([whether copysignf can be used without linking with libm], [gl_cv_func_copysignf_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include float x, y;]], [[return copysignf (x, y) < 0;]])], [gl_cv_func_copysignf_no_libm=yes], [gl_cv_func_copysignf_no_libm=no]) ]) if test $gl_cv_func_copysignf_no_libm = yes; then AC_DEFINE([HAVE_COPYSIGNF_IN_LIBC], [1], [Define if the copysignf function is declared in and available in libc.]) fi fi fi if test "$gl_cv_cc_double_signbit" = unknown; then dnl Test whether copysign() is declared. AC_CHECK_DECLS([copysign], , , [[#include ]]) if test "$ac_cv_have_decl_copysign" = yes; then dnl Test whether copysign() can be used without libm. AC_CACHE_CHECK([whether copysign can be used without linking with libm], [gl_cv_func_copysign_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include double x, y;]], [[return copysign (x, y) < 0;]])], [gl_cv_func_copysign_no_libm=yes], [gl_cv_func_copysign_no_libm=no]) ]) if test $gl_cv_func_copysign_no_libm = yes; then AC_DEFINE([HAVE_COPYSIGN_IN_LIBC], [1], [Define if the copysign function is declared in and available in libc.]) fi fi fi if test "$gl_cv_cc_long_double_signbit" = unknown; then dnl Test whether copysignl() is declared. AC_CHECK_DECLS([copysignl], , , [[#include ]]) if test "$ac_cv_have_decl_copysignl" = yes; then dnl Test whether copysignl() can be used without libm. AC_CACHE_CHECK([whether copysignl can be used without linking with libm], [gl_cv_func_copysignl_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include long double x, y;]], [[return copysignl (x, y) < 0;]])], [gl_cv_func_copysignl_no_libm=yes], [gl_cv_func_copysignl_no_libm=no]) ]) if test $gl_cv_func_copysignl_no_libm = yes; then AC_DEFINE([HAVE_COPYSIGNL_IN_LIBC], [1], [Define if the copysignl function is declared in and available in libc.]) fi fi fi ;; esac ;; esac ]) AC_DEFUN([gl_SIGNBIT_TEST_PROGRAM], [[ /* Global variables. Needed because GCC 4 constant-folds __builtin_signbitl (literal) but cannot constant-fold __builtin_signbitl (variable). */ float vf; double vd; long double vl; int main () { /* HP cc on HP-UX 10.20 has a bug with the constant expression -0.0. So we use -p0f and -p0d instead. */ float p0f = 0.0f; float m0f = -p0f; double p0d = 0.0; double m0d = -p0d; /* On HP-UX 10.20, negating 0.0L does not yield -0.0L. So we use another constant expression instead. But that expression does not work on other platforms, such as when cross-compiling to PowerPC on Mac OS X 10.5. */ long double p0l = 0.0L; #if defined __hpux || defined __sgi long double m0l = -LDBL_MIN * LDBL_MIN; #else long double m0l = -p0l; #endif int result = 0; if (signbit (vf)) /* link check */ vf++; { float plus_inf = 1.0f / p0f; float minus_inf = -1.0f / p0f; if (!(!signbit (255.0f) && signbit (-255.0f) && !signbit (p0f) && (memcmp (&m0f, &p0f, sizeof (float)) == 0 || signbit (m0f)) && !signbit (plus_inf) && signbit (minus_inf))) result |= 1; } if (signbit (vd)) /* link check */ vd++; { double plus_inf = 1.0 / p0d; double minus_inf = -1.0 / p0d; if (!(!signbit (255.0) && signbit (-255.0) && !signbit (p0d) && (memcmp (&m0d, &p0d, sizeof (double)) == 0 || signbit (m0d)) && !signbit (plus_inf) && signbit (minus_inf))) result |= 2; } if (signbit (vl)) /* link check */ vl++; { long double plus_inf = 1.0L / p0l; long double minus_inf = -1.0L / p0l; if (signbit (255.0L)) result |= 4; if (!signbit (-255.0L)) result |= 4; if (signbit (p0l)) result |= 8; if (!(memcmp (&m0l, &p0l, sizeof (long double)) == 0 || signbit (m0l))) result |= 16; if (signbit (plus_inf)) result |= 32; if (!signbit (minus_inf)) result |= 64; } return result; } ]]) AC_DEFUN([gl_FLOAT_SIGN_LOCATION], [ gl_FLOATTYPE_SIGN_LOCATION([float], [gl_cv_cc_float_signbit], [f], [FLT]) ]) AC_DEFUN([gl_DOUBLE_SIGN_LOCATION], [ gl_FLOATTYPE_SIGN_LOCATION([double], [gl_cv_cc_double_signbit], [], [DBL]) ]) AC_DEFUN([gl_LONG_DOUBLE_SIGN_LOCATION], [ gl_FLOATTYPE_SIGN_LOCATION([long double], [gl_cv_cc_long_double_signbit], [L], [LDBL]) ]) AC_DEFUN([gl_FLOATTYPE_SIGN_LOCATION], [ AC_CACHE_CHECK([where to find the sign bit in a '$1'], [$2], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #define NWORDS \ ((sizeof ($1) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { $1 value; unsigned int word[NWORDS]; } memory_float; static memory_float plus = { 1.0$3 }; static memory_float minus = { -1.0$3 }; int main () { size_t j, k, i; unsigned int m; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; /* Find the different bit. */ k = 0; m = 0; for (j = 0; j < NWORDS; j++) { unsigned int x = plus.word[j] ^ minus.word[j]; if ((x & (x - 1)) || (x && m)) { /* More than one bit difference. */ fprintf (fp, "unknown"); fclose (fp); return 2; } if (x) { k = j; m = x; } } if (m == 0) { /* No difference. */ fprintf (fp, "unknown"); fclose (fp); return 3; } /* Now m = plus.word[k] ^ ~minus.word[k]. */ if (plus.word[k] & ~minus.word[k]) { /* Oh? The sign bit is set in the positive and cleared in the negative numbers? */ fprintf (fp, "unknown"); fclose (fp); return 4; } for (i = 0; ; i++) if ((m >> i) & 1) break; fprintf (fp, "word %d bit %d", (int) k, (int) i); if (fclose (fp) != 0) return 5; return 0; } ]])], [$2=`cat conftest.out`], [$2="unknown"], [ dnl When cross-compiling, we don't know. It depends on the dnl ABI and compiler version. There are too many cases. $2="unknown" ]) rm -f conftest.out ]) case "$]$2[" in word*bit*) word=`echo "$]$2[" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$]$2[" | sed -e 's/word.*bit //'` AC_DEFINE_UNQUOTED([$4][_SIGNBIT_WORD], [$word], [Define as the word index where to find the sign of '$1'.]) AC_DEFINE_UNQUOTED([$4][_SIGNBIT_BIT], [$bit], [Define as the bit index in the word where to find the sign of '$1'.]) ;; esac ]) # Expands to code that defines a function signbitf(float). # It extracts the sign bit of a non-NaN value. AC_DEFUN([gl_FLOAT_SIGNBIT_CODE], [ gl_FLOATTYPE_SIGNBIT_CODE([float], [f], [f]) ]) # Expands to code that defines a function signbitd(double). # It extracts the sign bit of a non-NaN value. AC_DEFUN([gl_DOUBLE_SIGNBIT_CODE], [ gl_FLOATTYPE_SIGNBIT_CODE([double], [d], []) ]) # Expands to code that defines a function signbitl(long double). # It extracts the sign bit of a non-NaN value. AC_DEFUN([gl_LONG_DOUBLE_SIGNBIT_CODE], [ gl_FLOATTYPE_SIGNBIT_CODE([long double], [l], [L]) ]) AC_DEFUN([gl_FLOATTYPE_SIGNBIT_CODE], [[ static int signbit$2 ($1 value) { typedef union { $1 f; unsigned char b[sizeof ($1)]; } float_union; static float_union plus_one = { 1.0$3 }; /* unused bits are zero here */ static float_union minus_one = { -1.0$3 }; /* unused bits are zero here */ /* Compute the sign bit mask as the XOR of plus_one and minus_one. */ float_union u; unsigned int i; u.f = value; for (i = 0; i < sizeof ($1); i++) if (u.b[i] & (plus_one.b[i] ^ minus_one.b[i])) return 1; return 0; } ]]) gnuastro-0.5/bootstrapped/m4/signalblocking.m40000644000175000017500000000164113217200022016406 00000000000000# signalblocking.m4 serial 14 dnl Copyright (C) 2001-2002, 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Determine available signal blocking primitives. Three different APIs exist: # 1) POSIX: sigemptyset, sigaddset, sigprocmask # 2) SYSV: sighold, sigrelse # 3) BSD: sigblock, sigsetmask # For simplicity, here we check only for the POSIX signal blocking. AC_DEFUN([gl_SIGNALBLOCKING], [ AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) AC_REQUIRE([gl_CHECK_TYPE_SIGSET_T]) if test $gl_cv_type_sigset_t = yes; then AC_CHECK_FUNC([sigprocmask], [gl_cv_func_sigprocmask=1]) fi if test -z "$gl_cv_func_sigprocmask"; then HAVE_POSIX_SIGNALBLOCKING=0 fi ]) # Prerequisites of lib/sigprocmask.c. AC_DEFUN([gl_PREREQ_SIGPROCMASK], [:]) gnuastro-0.5/bootstrapped/m4/signal_h.m40000644000175000017500000000604213217200022015204 00000000000000# signal_h.m4 serial 18 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_SIGNAL_H], [ AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) AC_REQUIRE([gl_CHECK_TYPE_SIGSET_T]) gl_NEXT_HEADERS([signal.h]) # AIX declares sig_atomic_t to already include volatile, and C89 compilers # then choke on 'volatile sig_atomic_t'. C99 requires that it compile. AC_CHECK_TYPE([volatile sig_atomic_t], [], [HAVE_TYPE_VOLATILE_SIG_ATOMIC_T=0], [[ #include ]]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) AC_REQUIRE([AC_TYPE_UID_T]) dnl Persuade glibc to define sighandler_t. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_TYPE([sighandler_t], [], [HAVE_SIGHANDLER_T=0], [[ #include ]]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [pthread_sigmask sigaction sigaddset sigdelset sigemptyset sigfillset sigismember sigpending sigprocmask]) ]) AC_DEFUN([gl_CHECK_TYPE_SIGSET_T], [ AC_CHECK_TYPES([sigset_t], [gl_cv_type_sigset_t=yes], [gl_cv_type_sigset_t=no], [[ #include /* Mingw defines sigset_t not in , but in . */ #include ]]) if test $gl_cv_type_sigset_t != yes; then HAVE_SIGSET_T=0 fi ]) AC_DEFUN([gl_SIGNAL_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_SIGNAL_H_DEFAULTS], [ GNULIB_PTHREAD_SIGMASK=0; AC_SUBST([GNULIB_PTHREAD_SIGMASK]) GNULIB_RAISE=0; AC_SUBST([GNULIB_RAISE]) GNULIB_SIGNAL_H_SIGPIPE=0; AC_SUBST([GNULIB_SIGNAL_H_SIGPIPE]) GNULIB_SIGPROCMASK=0; AC_SUBST([GNULIB_SIGPROCMASK]) GNULIB_SIGACTION=0; AC_SUBST([GNULIB_SIGACTION]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_POSIX_SIGNALBLOCKING=1; AC_SUBST([HAVE_POSIX_SIGNALBLOCKING]) HAVE_PTHREAD_SIGMASK=1; AC_SUBST([HAVE_PTHREAD_SIGMASK]) HAVE_RAISE=1; AC_SUBST([HAVE_RAISE]) HAVE_SIGSET_T=1; AC_SUBST([HAVE_SIGSET_T]) HAVE_SIGINFO_T=1; AC_SUBST([HAVE_SIGINFO_T]) HAVE_SIGACTION=1; AC_SUBST([HAVE_SIGACTION]) HAVE_STRUCT_SIGACTION_SA_SIGACTION=1; AC_SUBST([HAVE_STRUCT_SIGACTION_SA_SIGACTION]) HAVE_TYPE_VOLATILE_SIG_ATOMIC_T=1; AC_SUBST([HAVE_TYPE_VOLATILE_SIG_ATOMIC_T]) HAVE_SIGHANDLER_T=1; AC_SUBST([HAVE_SIGHANDLER_T]) REPLACE_PTHREAD_SIGMASK=0; AC_SUBST([REPLACE_PTHREAD_SIGMASK]) REPLACE_RAISE=0; AC_SUBST([REPLACE_RAISE]) ]) gnuastro-0.5/bootstrapped/m4/sigaction.m40000644000175000017500000000232513217200022015400 00000000000000# sigaction.m4 serial 7 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Determine if sigaction interface is present. AC_DEFUN([gl_SIGACTION], [ AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([sigaction]) if test $ac_cv_func_sigaction = yes; then AC_CHECK_MEMBERS([struct sigaction.sa_sigaction], , , [[#include ]]) if test $ac_cv_member_struct_sigaction_sa_sigaction = no; then HAVE_STRUCT_SIGACTION_SA_SIGACTION=0 fi else HAVE_SIGACTION=0 fi ]) # Prerequisites of the part of lib/signal.in.h and of lib/sigaction.c. AC_DEFUN([gl_PREREQ_SIGACTION], [ AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([AC_TYPE_UID_T]) AC_REQUIRE([gl_PREREQ_SIG_HANDLER_H]) AC_CHECK_FUNCS_ONCE([sigaltstack siginterrupt]) AC_CHECK_TYPES([siginfo_t], [], [], [[ #include ]]) if test $ac_cv_type_siginfo_t = no; then HAVE_SIGINFO_T=0 fi ]) # Prerequisites of lib/sig-handler.h. AC_DEFUN([gl_PREREQ_SIG_HANDLER_H], [:]) gnuastro-0.5/bootstrapped/m4/setlocale.m40000644000175000017500000000154313217200022015374 00000000000000# setlocale.m4 serial 4 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SETLOCALE], [ AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in dnl On native Windows systems, setlocale(category,NULL) does not look at dnl the environment variables LC_ALL, category, and LANG. mingw*) REPLACE_SETLOCALE=1 ;; dnl On Cygwin 1.5.x, setlocale always succeeds but setlocale(LC_CTYPE,NULL) dnl is then still "C". cygwin*) case `uname -r` in 1.5.*) REPLACE_SETLOCALE=1 ;; esac ;; esac ]) # Prerequisites of lib/setlocale.c. AC_DEFUN([gl_PREREQ_SETLOCALE], [ : ]) gnuastro-0.5/bootstrapped/m4/setenv.m40000644000175000017500000001101213217200022014715 00000000000000# setenv.m4 serial 26 dnl Copyright (C) 2001-2004, 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SETENV], [ AC_REQUIRE([gl_FUNC_SETENV_SEPARATE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles if test $ac_cv_func_setenv = no; then HAVE_SETENV=0 else AC_CACHE_CHECK([whether setenv validates arguments], [gl_cv_func_setenv_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include #include ]], [[ int result = 0; { if (setenv ("", "", 0) != -1) result |= 1; else if (errno != EINVAL) result |= 2; } { if (setenv ("a", "=", 1) != 0) result |= 4; else if (strcmp (getenv ("a"), "=") != 0) result |= 8; } return result; ]])], [gl_cv_func_setenv_works=yes], [gl_cv_func_setenv_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_setenv_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_setenv_works="guessing no" ;; esac ])]) case "$gl_cv_func_setenv_works" in *yes) ;; *) REPLACE_SETENV=1 ;; esac fi ]) # Like gl_FUNC_SETENV, except prepare for separate compilation # (no REPLACE_SETENV, no AC_LIBOBJ). AC_DEFUN([gl_FUNC_SETENV_SEPARATE], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_CHECK_DECLS_ONCE([setenv]) if test $ac_cv_have_decl_setenv = no; then HAVE_DECL_SETENV=0 fi AC_CHECK_FUNCS_ONCE([setenv]) gl_PREREQ_SETENV ]) AC_DEFUN([gl_FUNC_UNSETENV], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_DECLS_ONCE([unsetenv]) if test $ac_cv_have_decl_unsetenv = no; then HAVE_DECL_UNSETENV=0 fi AC_CHECK_FUNCS([unsetenv]) if test $ac_cv_func_unsetenv = no; then HAVE_UNSETENV=0 else HAVE_UNSETENV=1 dnl Some BSDs return void, failing to do error checking. AC_CACHE_CHECK([for unsetenv() return type], [gt_cv_func_unsetenv_ret], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #undef _BSD #define _BSD 1 /* unhide unsetenv declaration in OSF/1 5.1 */ #include extern #ifdef __cplusplus "C" #endif int unsetenv (const char *name); ]], [[]])], [gt_cv_func_unsetenv_ret='int'], [gt_cv_func_unsetenv_ret='void'])]) if test $gt_cv_func_unsetenv_ret = 'void'; then AC_DEFINE([VOID_UNSETENV], [1], [Define to 1 if unsetenv returns void instead of int.]) REPLACE_UNSETENV=1 fi dnl Solaris 10 unsetenv does not remove all copies of a name. dnl Haiku alpha 2 unsetenv gets confused by assignment to environ. dnl OpenBSD 4.7 unsetenv("") does not fail. AC_CACHE_CHECK([whether unsetenv obeys POSIX], [gl_cv_func_unsetenv_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include extern char **environ; ]], [[ char entry1[] = "a=1"; char entry2[] = "b=2"; char *env[] = { entry1, entry2, NULL }; if (putenv ((char *) "a=1")) return 1; if (putenv (entry2)) return 2; entry2[0] = 'a'; unsetenv ("a"); if (getenv ("a")) return 3; if (!unsetenv ("") || errno != EINVAL) return 4; entry2[0] = 'b'; environ = env; if (!getenv ("a")) return 5; entry2[0] = 'a'; unsetenv ("a"); if (getenv ("a")) return 6; ]])], [gl_cv_func_unsetenv_works=yes], [gl_cv_func_unsetenv_works=no], [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_unsetenv_works="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_unsetenv_works="guessing no" ;; esac ])]) case "$gl_cv_func_unsetenv_works" in *yes) ;; *) REPLACE_UNSETENV=1 ;; esac fi ]) # Prerequisites of lib/setenv.c. AC_DEFUN([gl_PREREQ_SETENV], [ AC_REQUIRE([AC_FUNC_ALLOCA]) AC_REQUIRE([gl_ENVIRON]) AC_CHECK_HEADERS_ONCE([unistd.h]) AC_CHECK_HEADERS([search.h]) AC_CHECK_FUNCS([tsearch]) ]) # Prerequisites of lib/unsetenv.c. AC_DEFUN([gl_PREREQ_UNSETENV], [ AC_REQUIRE([gl_ENVIRON]) AC_CHECK_HEADERS_ONCE([unistd.h]) ]) gnuastro-0.5/bootstrapped/m4/select.m40000644000175000017500000000634413217200022014704 00000000000000# select.m4 serial 8 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_SELECT], [ AC_REQUIRE([gl_HEADER_SYS_SELECT]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SOCKETS]) if test "$ac_cv_header_winsock2_h" = yes; then REPLACE_SELECT=1 else dnl On Interix 3.5, select(0, NULL, NULL, NULL, timeout) fails with error dnl EFAULT. AC_CHECK_HEADERS_ONCE([sys/select.h]) AC_CACHE_CHECK([whether select supports a 0 argument], [gl_cv_func_select_supports0], [ AC_RUN_IFELSE([AC_LANG_SOURCE([[ #include #include #if HAVE_SYS_SELECT_H #include #endif int main () { struct timeval timeout; timeout.tv_sec = 0; timeout.tv_usec = 5; return select (0, (fd_set *)0, (fd_set *)0, (fd_set *)0, &timeout) < 0; }]])], [gl_cv_func_select_supports0=yes], [gl_cv_func_select_supports0=no], [ changequote(,)dnl case "$host_os" in # Guess no on Interix. interix*) gl_cv_func_select_supports0="guessing no";; # Guess yes otherwise. *) gl_cv_func_select_supports0="guessing yes";; esac changequote([,])dnl ]) ]) case "$gl_cv_func_select_supports0" in *yes) ;; *) REPLACE_SELECT=1 ;; esac dnl On FreeBSD 8.2, select() doesn't always reject bad fds. AC_CACHE_CHECK([whether select detects invalid fds], [gl_cv_func_select_detects_ebadf], [ AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #include #if HAVE_SYS_SELECT_H # include #endif #include #include ]],[[ fd_set set; dup2(0, 16); FD_ZERO(&set); FD_SET(16, &set); close(16); struct timeval timeout; timeout.tv_sec = 0; timeout.tv_usec = 5; return select (17, &set, NULL, NULL, &timeout) != -1 || errno != EBADF; ]])], [gl_cv_func_select_detects_ebadf=yes], [gl_cv_func_select_detects_ebadf=no], [ case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_select_detects_ebadf="guessing yes" ;; # If we don't know, assume the worst. *) gl_cv_func_select_detects_ebadf="guessing no" ;; esac ]) ]) case $gl_cv_func_select_detects_ebadf in *yes) ;; *) REPLACE_SELECT=1 ;; esac fi dnl Determine the needed libraries. LIB_SELECT="$LIBSOCKET" if test $REPLACE_SELECT = 1; then case "$host_os" in mingw*) dnl On the MSVC platform, the function MsgWaitForMultipleObjects dnl (used in lib/select.c) requires linking with -luser32. On mingw, dnl it is implicit. AC_LINK_IFELSE( [AC_LANG_SOURCE([[ #define WIN32_LEAN_AND_MEAN #include int main () { MsgWaitForMultipleObjects (0, NULL, 0, 0, 0); return 0; }]])], [], [LIB_SELECT="$LIB_SELECT -luser32"]) ;; esac fi AC_SUBST([LIB_SELECT]) ]) gnuastro-0.5/bootstrapped/m4/regex.m40000644000175000017500000002767413217200022014550 00000000000000# serial 67 # Copyright (C) 1996-2001, 2003-2017 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl Initially derived from code in GNU grep. dnl Mostly written by Jim Meyering. AC_PREREQ([2.50]) AC_DEFUN([gl_REGEX], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_ARG_WITH([included-regex], [AS_HELP_STRING([--without-included-regex], [don't compile regex; this is the default on systems with recent-enough versions of the GNU C Library (use with caution on other systems).])]) case $with_included_regex in #( yes|no) ac_use_included_regex=$with_included_regex ;; '') # If the system regex support is good enough that it passes the # following run test, then default to *not* using the included regex.c. # If cross compiling, assume the test would fail and use the included # regex.c. AC_CHECK_DECLS_ONCE([alarm]) AC_CHECK_HEADERS_ONCE([malloc.h]) AC_CACHE_CHECK([for working re_compile_pattern], [gl_cv_func_re_compile_pattern_working], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include #include #if defined M_CHECK_ACTION || HAVE_DECL_ALARM # include # include #endif #if HAVE_MALLOC_H # include #endif #ifdef M_CHECK_ACTION /* Exit with distinguishable exit code. */ static void sigabrt_no_core (int sig) { raise (SIGTERM); } #endif ]], [[int result = 0; static struct re_pattern_buffer regex; unsigned char folded_chars[UCHAR_MAX + 1]; int i; const char *s; struct re_registers regs; /* Some builds of glibc go into an infinite loop on this test. Use alarm to force death, and mallopt to avoid malloc recursion in diagnosing the corrupted heap. */ #if HAVE_DECL_ALARM signal (SIGALRM, SIG_DFL); alarm (2); #endif #ifdef M_CHECK_ACTION signal (SIGABRT, sigabrt_no_core); mallopt (M_CHECK_ACTION, 2); #endif if (setlocale (LC_ALL, "en_US.UTF-8")) { { /* https://sourceware.org/ml/libc-hacker/2006-09/msg00008.html This test needs valgrind to catch the bug on Debian GNU/Linux 3.1 x86, but it might catch the bug better on other platforms and it shouldn't hurt to try the test here. */ static char const pat[] = "insert into"; static char const data[] = "\xFF\0\x12\xA2\xAA\xC4\xB1,K\x12\xC4\xB1*\xACK"; re_set_syntax (RE_SYNTAX_GREP | RE_HAT_LISTS_NOT_NEWLINE | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else if (re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, ®s) != -1) result |= 1; regfree (®ex); } { /* This test is from glibc bug 15078. The test case is from Andreas Schwab in . */ static char const pat[] = "[^x]x"; static char const data[] = /* */ "\xe1\x80\x80" "\xe1\x80\xbb" "\xe1\x80\xbd" "\xe1\x80\x94" "\xe1\x80\xba" "\xe1\x80\xaf" "\xe1\x80\x95" "\xe1\x80\xba" "x"; re_set_syntax (0); memset (®ex, 0, sizeof regex); s = re_compile_pattern (pat, sizeof pat - 1, ®ex); if (s) result |= 1; else { i = re_search (®ex, data, sizeof data - 1, 0, sizeof data - 1, 0); if (i != 0 && i != 21) result |= 1; } regfree (®ex); } if (! setlocale (LC_ALL, "C")) return 1; } /* This test is from glibc bug 3957, reported by Andrew Mackey. */ re_set_syntax (RE_SYNTAX_EGREP | RE_HAT_LISTS_NOT_NEWLINE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[^x]b", 6, ®ex); if (s) result |= 2; /* This should fail, but succeeds for glibc-2.5. */ else if (re_search (®ex, "a\nb", 3, 0, 3, ®s) != -1) result |= 2; /* This regular expression is from Spencer ere test number 75 in grep-2.3. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP); memset (®ex, 0, sizeof regex); for (i = 0; i <= UCHAR_MAX; i++) folded_chars[i] = i; regex.translate = folded_chars; s = re_compile_pattern ("a[[:@:>@:]]b\n", 11, ®ex); /* This should fail with _Invalid character class name_ error. */ if (!s) result |= 4; /* Ensure that [b-a] is diagnosed as invalid, when using RE_NO_EMPTY_RANGES. */ re_set_syntax (RE_SYNTAX_POSIX_EGREP | RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("a[b-a]", 6, ®ex); if (s == 0) result |= 8; /* This should succeed, but does not for glibc-2.1.3. */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("{1", 2, ®ex); if (s) result |= 8; /* The following example is derived from a problem report against gawk from Jorge Stolfi . */ memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[an\371]*n", 7, ®ex); if (s) result |= 8; /* This should match, but does not for glibc-2.2.1. */ else if (re_match (®ex, "an", 2, 0, ®s) != 2) result |= 8; memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 8; /* glibc-2.2.93 does not work with a negative RANGE argument. */ else if (re_search (®ex, "wxy", 3, 2, -2, ®s) != 1) result |= 8; /* The version of regex.c in older versions of gnulib ignored RE_ICASE. Detect that problem too. */ re_set_syntax (RE_SYNTAX_EMACS | RE_ICASE); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("x", 1, ®ex); if (s) result |= 16; else if (re_search (®ex, "WXY", 3, 0, 3, ®s) < 0) result |= 16; /* Catch a bug reported by Vin Shelton in https://lists.gnu.org/r/bug-coreutils/2007-06/msg00089.html */ re_set_syntax (RE_SYNTAX_POSIX_BASIC & ~RE_CONTEXT_INVALID_DUP & ~RE_NO_EMPTY_RANGES); memset (®ex, 0, sizeof regex); s = re_compile_pattern ("[[:alnum:]_-]\\\\+$", 16, ®ex); if (s) result |= 32; /* REG_STARTEND was added to glibc on 2004-01-15. Reject older versions. */ if (! REG_STARTEND) result |= 64; #if 0 /* It would be nice to reject hosts whose regoff_t values are too narrow (including glibc on hosts with 64-bit ptrdiff_t and 32-bit int), but we should wait until glibc implements this feature. Otherwise, support for equivalence classes and multibyte collation symbols would always be broken except when compiling --without-included-regex. */ if (sizeof (regoff_t) < sizeof (ptrdiff_t) || sizeof (regoff_t) < sizeof (ssize_t)) result |= 64; #endif return result; ]])], [gl_cv_func_re_compile_pattern_working=yes], [gl_cv_func_re_compile_pattern_working=no], [case "$host_os" in # Guess no on native Windows. mingw*) gl_cv_func_re_compile_pattern_working="guessing no" ;; # Otherwise, assume it is not working. *) gl_cv_func_re_compile_pattern_working="guessing no" ;; esac ]) ]) case "$gl_cv_func_re_compile_pattern_working" in #( *yes) ac_use_included_regex=no;; #( *no) ac_use_included_regex=yes;; esac ;; *) AC_MSG_ERROR([Invalid value for --with-included-regex: $with_included_regex]) ;; esac if test $ac_use_included_regex = yes; then AC_DEFINE([_REGEX_INCLUDE_LIMITS_H], [1], [Define if you want to include , so that it consistently overrides 's RE_DUP_MAX.]) AC_DEFINE([_REGEX_LARGE_OFFSETS], [1], [Define if you want regoff_t to be at least as wide POSIX requires.]) AC_DEFINE([re_syntax_options], [rpl_re_syntax_options], [Define to rpl_re_syntax_options if the replacement should be used.]) AC_DEFINE([re_set_syntax], [rpl_re_set_syntax], [Define to rpl_re_set_syntax if the replacement should be used.]) AC_DEFINE([re_compile_pattern], [rpl_re_compile_pattern], [Define to rpl_re_compile_pattern if the replacement should be used.]) AC_DEFINE([re_compile_fastmap], [rpl_re_compile_fastmap], [Define to rpl_re_compile_fastmap if the replacement should be used.]) AC_DEFINE([re_search], [rpl_re_search], [Define to rpl_re_search if the replacement should be used.]) AC_DEFINE([re_search_2], [rpl_re_search_2], [Define to rpl_re_search_2 if the replacement should be used.]) AC_DEFINE([re_match], [rpl_re_match], [Define to rpl_re_match if the replacement should be used.]) AC_DEFINE([re_match_2], [rpl_re_match_2], [Define to rpl_re_match_2 if the replacement should be used.]) AC_DEFINE([re_set_registers], [rpl_re_set_registers], [Define to rpl_re_set_registers if the replacement should be used.]) AC_DEFINE([re_comp], [rpl_re_comp], [Define to rpl_re_comp if the replacement should be used.]) AC_DEFINE([re_exec], [rpl_re_exec], [Define to rpl_re_exec if the replacement should be used.]) AC_DEFINE([regcomp], [rpl_regcomp], [Define to rpl_regcomp if the replacement should be used.]) AC_DEFINE([regexec], [rpl_regexec], [Define to rpl_regexec if the replacement should be used.]) AC_DEFINE([regerror], [rpl_regerror], [Define to rpl_regerror if the replacement should be used.]) AC_DEFINE([regfree], [rpl_regfree], [Define to rpl_regfree if the replacement should be used.]) fi ]) # Prerequisites of lib/regex.c and lib/regex_internal.c. AC_DEFUN([gl_PREREQ_REGEX], [ AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([AC_C_INLINE]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) AC_REQUIRE([gl_EEMALLOC]) AC_REQUIRE([gl_GLIBC21]) AC_CHECK_HEADERS([libintl.h]) AC_CHECK_FUNCS_ONCE([isblank iswctype]) AC_CHECK_DECLS([isblank], [], [], [[#include ]]) ]) gnuastro-0.5/bootstrapped/m4/rawmemchr.m40000644000175000017500000000117213217200022015404 00000000000000# rawmemchr.m4 serial 2 dnl Copyright (C) 2003, 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_RAWMEMCHR], [ dnl Persuade glibc to declare rawmemchr(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_FUNCS([rawmemchr]) if test $ac_cv_func_rawmemchr = no; then HAVE_RAWMEMCHR=0 fi ]) # Prerequisites of lib/strchrnul.c. AC_DEFUN([gl_PREREQ_RAWMEMCHR], [:]) gnuastro-0.5/bootstrapped/m4/raise.m40000644000175000017500000000177113217200022014527 00000000000000# raise.m4 serial 4 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_RAISE], [ AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS([raise]) if test $ac_cv_func_raise = no; then HAVE_RAISE=0 else m4_ifdef([gl_MSVC_INVAL], [ AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_RAISE=1 fi ]) m4_ifdef([gl_SIGNALBLOCKING], [ gl_SIGNALBLOCKING if test $HAVE_POSIX_SIGNALBLOCKING = 0; then m4_ifdef([gl_SIGNAL_SIGPIPE], [ gl_SIGNAL_SIGPIPE if test $gl_cv_header_signal_h_SIGPIPE != yes; then REPLACE_RAISE=1 fi ], [:]) fi ]) fi ]) # Prerequisites of lib/raise.c. AC_DEFUN([gl_PREREQ_RAISE], [:]) gnuastro-0.5/bootstrapped/m4/putenv.m40000644000175000017500000000336313217200022014744 00000000000000# putenv.m4 serial 21 dnl Copyright (C) 2002-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Jim Meyering. dnl dnl Check whether putenv ("FOO") removes FOO from the environment. dnl The putenv in libc on at least SunOS 4.1.4 does *not* do that. AC_DEFUN([gl_FUNC_PUTENV], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([for putenv compatible with GNU and SVID], [gl_cv_func_svid_putenv], [AC_RUN_IFELSE([AC_LANG_PROGRAM([AC_INCLUDES_DEFAULT],[[ /* Put it in env. */ if (putenv ("CONFTEST_putenv=val")) return 1; /* Try to remove it. */ if (putenv ("CONFTEST_putenv")) return 2; /* Make sure it was deleted. */ if (getenv ("CONFTEST_putenv") != 0) return 3; return 0; ]])], gl_cv_func_svid_putenv=yes, gl_cv_func_svid_putenv=no, dnl When crosscompiling, assume putenv is broken. [case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_svid_putenv="guessing yes" ;; # Guess no on native Windows. mingw*) gl_cv_func_svid_putenv="guessing no" ;; # If we don't know, assume the worst. *) gl_cv_func_svid_putenv="guessing no" ;; esac ]) ]) case "$gl_cv_func_svid_putenv" in *yes) ;; *) REPLACE_PUTENV=1 ;; esac ]) # Prerequisites of lib/putenv.c. AC_DEFUN([gl_PREREQ_PUTENV], [ AC_CHECK_DECLS([_putenv]) ]) gnuastro-0.5/bootstrapped/m4/pthread_sigmask.m40000644000175000017500000002307413217200022016571 00000000000000# pthread_sigmask.m4 serial 16 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_PTHREAD_SIGMASK], [ AC_REQUIRE([gl_SIGNAL_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([pthread_sigmask]) LIB_PTHREAD_SIGMASK= dnl Test whether the gnulib module 'threadlib' is in use. dnl Some packages like Emacs use --avoid=threadlib. dnl Write the symbol in such a way that it does not cause 'aclocal' to pick dnl the threadlib.m4 file that is installed in $PREFIX/share/aclocal/. m4_ifdef([gl_][THREADLIB], [ AC_REQUIRE([gl_][THREADLIB]) if test "$gl_threads_api" = posix; then if test $ac_cv_func_pthread_sigmask = yes; then dnl pthread_sigmask is available without -lpthread. : else if test -n "$LIBMULTITHREAD"; then AC_CACHE_CHECK([for pthread_sigmask in $LIBMULTITHREAD], [gl_cv_func_pthread_sigmask_in_LIBMULTITHREAD], [gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[return pthread_sigmask (0, (sigset_t *) 0, (sigset_t *) 0);]]) ], [gl_cv_func_pthread_sigmask_in_LIBMULTITHREAD=yes], [gl_cv_func_pthread_sigmask_in_LIBMULTITHREAD=no]) LIBS="$gl_save_LIBS" ]) if test $gl_cv_func_pthread_sigmask_in_LIBMULTITHREAD = yes; then AC_CACHE_CHECK([whether pthread_sigmask is only a macro], [gl_cv_func_pthread_sigmask_is_macro], [gl_save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #include #undef pthread_sigmask ]], [[return pthread_sigmask (0, (sigset_t *) 0, (sigset_t *) 0);]]) ], [gl_cv_func_pthread_sigmask_is_macro=no], [gl_cv_func_pthread_sigmask_is_macro=yes]) LIBS="$gl_save_LIBS" ]) if test $gl_cv_func_pthread_sigmask_is_macro = yes; then dnl On MinGW pthread_sigmask is just a macro which always returns 0. dnl It does not exist as a real function, which is required by POSIX. REPLACE_PTHREAD_SIGMASK=1 gl_cv_func_pthread_sigmask_in_LIBMULTITHREAD=no fi fi if test $gl_cv_func_pthread_sigmask_in_LIBMULTITHREAD = yes; then dnl pthread_sigmask is available with -pthread or -lpthread. LIB_PTHREAD_SIGMASK="$LIBMULTITHREAD" else dnl pthread_sigmask is not available at all. HAVE_PTHREAD_SIGMASK=0 fi else dnl pthread_sigmask is not available at all. HAVE_PTHREAD_SIGMASK=0 fi fi else dnl pthread_sigmask may exist but does not interoperate with the chosen dnl multithreading facility. dnl If "$gl_threads_api" = pth, we could use the function pth_sigmask, dnl but it is equivalent to sigprocmask, so we choose to emulate dnl pthread_sigmask with sigprocmask also in this case. This yields fewer dnl link dependencies. if test $ac_cv_func_pthread_sigmask = yes; then REPLACE_PTHREAD_SIGMASK=1 else HAVE_PTHREAD_SIGMASK=0 fi fi ], [ dnl The module 'threadlib' is not in use, due to --avoid=threadlib being dnl specified. dnl The package either has prepared CPPFLAGS and LIBS for use of POSIX:2008 dnl threads, or wants to build single-threaded programs. if test $ac_cv_func_pthread_sigmask = yes; then dnl pthread_sigmask exists and does not require extra libraries. dnl Assume that it is declared. : else dnl pthread_sigmask either does not exist or needs extra libraries. HAVE_PTHREAD_SIGMASK=0 dnl Define the symbol rpl_pthread_sigmask, not pthread_sigmask, dnl so as to not accidentally override the system's pthread_sigmask dnl symbol from libpthread. This is necessary on IRIX 6.5. REPLACE_PTHREAD_SIGMASK=1 fi ]) AC_SUBST([LIB_PTHREAD_SIGMASK]) dnl We don't need a variable LTLIB_PTHREAD_SIGMASK, because when dnl "$gl_threads_api" = posix, $LTLIBMULTITHREAD and $LIBMULTITHREAD are the dnl same. dnl Now test for some bugs in the system function. if test $HAVE_PTHREAD_SIGMASK = 1; then AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl On FreeBSD 6.4, HP-UX 11.31, Solaris 9, in programs that are not linked dnl with -lpthread, the pthread_sigmask() function always returns 0 and has dnl no effect. if test -z "$LIB_PTHREAD_SIGMASK"; then case " $LIBS " in *' -pthread '*) ;; *' -lpthread '*) ;; *) AC_CACHE_CHECK([whether pthread_sigmask works without -lpthread], [gl_cv_func_pthread_sigmask_in_libc_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { sigset_t set; sigemptyset (&set); return pthread_sigmask (1729, &set, NULL) != 0; }]])], [gl_cv_func_pthread_sigmask_in_libc_works=no], [gl_cv_func_pthread_sigmask_in_libc_works=yes], [ changequote(,)dnl case "$host_os" in freebsd* | hpux* | solaris | solaris2.[2-9]*) gl_cv_func_pthread_sigmask_in_libc_works="guessing no";; *) gl_cv_func_pthread_sigmask_in_libc_works="guessing yes";; esac changequote([,])dnl ]) ]) case "$gl_cv_func_pthread_sigmask_in_libc_works" in *no) REPLACE_PTHREAD_SIGMASK=1 AC_DEFINE([PTHREAD_SIGMASK_INEFFECTIVE], [1], [Define to 1 if pthread_sigmask may return 0 and have no effect.]) ;; esac;; esac fi dnl On Cygwin 1.7.5, the pthread_sigmask() has a wrong return value dnl convention: Upon failure, it returns -1 and sets errno. AC_CACHE_CHECK([whether pthread_sigmask returns error numbers], [gl_cv_func_pthread_sigmask_return_works], [ gl_save_LIBS="$LIBS" LIBS="$LIBS $LIB_PTHREAD_SIGMASK" AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { sigset_t set; sigemptyset (&set); if (pthread_sigmask (1729, &set, NULL) == -1) return 1; return 0; }]])], [gl_cv_func_pthread_sigmask_return_works=yes], [gl_cv_func_pthread_sigmask_return_works=no], [case "$host_os" in cygwin*) gl_cv_func_pthread_sigmask_return_works="guessing no";; *) gl_cv_func_pthread_sigmask_return_works="guessing yes";; esac ]) LIBS="$gl_save_LIBS" ]) case "$gl_cv_func_pthread_sigmask_return_works" in *no) REPLACE_PTHREAD_SIGMASK=1 AC_DEFINE([PTHREAD_SIGMASK_FAILS_WITH_ERRNO], [1], [Define to 1 if pthread_sigmask(), when it fails, returns -1 and sets errno.]) ;; esac dnl On IRIX 6.5, in a single-threaded program, pending signals are not dnl immediately delivered when they are unblocked through pthread_sigmask, dnl only a little while later. AC_CACHE_CHECK([whether pthread_sigmask unblocks signals correctly], [gl_cv_func_pthread_sigmask_unblock_works], [ case "$host_os" in irix*) gl_cv_func_pthread_sigmask_unblock_works="guessing no";; *) gl_cv_func_pthread_sigmask_unblock_works="guessing yes";; esac m4_ifdef([gl_][THREADLIB], [dnl Link against $LIBMULTITHREAD, not only $LIB_PTHREAD_SIGMASK. dnl Otherwise we get a false positive on those platforms where dnl $gl_cv_func_pthread_sigmask_in_libc_works is "no". gl_save_LIBS=$LIBS LIBS="$LIBS $LIBMULTITHREAD"]) AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #include static volatile int sigint_occurred; static void sigint_handler (int sig) { sigint_occurred++; } int main () { sigset_t set; int pid = getpid (); char command[80]; signal (SIGINT, sigint_handler); sigemptyset (&set); sigaddset (&set, SIGINT); if (!(pthread_sigmask (SIG_BLOCK, &set, NULL) == 0)) return 1; sprintf (command, "sh -c 'sleep 1; kill -%d %d' &", SIGINT, pid); if (!(system (command) == 0)) return 2; sleep (2); if (!(sigint_occurred == 0)) return 3; if (!(pthread_sigmask (SIG_UNBLOCK, &set, NULL) == 0)) return 4; if (!(sigint_occurred == 1)) /* This fails on IRIX. */ return 5; return 0; }]])], [:], [gl_cv_func_pthread_sigmask_unblock_works=no], [:]) m4_ifdef([gl_][THREADLIB], [LIBS=$gl_save_LIBS]) ]) case "$gl_cv_func_pthread_sigmask_unblock_works" in *no) REPLACE_PTHREAD_SIGMASK=1 AC_DEFINE([PTHREAD_SIGMASK_UNBLOCK_BUG], [1], [Define to 1 if pthread_sigmask() unblocks signals incorrectly.]) ;; esac fi ]) # Prerequisite of lib/pthread_sigmask.c. AC_DEFUN([gl_PREREQ_PTHREAD_SIGMASK], [ if test $HAVE_PTHREAD_SIGMASK = 1; then AC_DEFINE([HAVE_PTHREAD_SIGMASK], [1], [Define to 1 if the pthread_sigmask function can be used (despite bugs).]) fi ]) gnuastro-0.5/bootstrapped/m4/pthread_rwlock_rdlock.m40000644000175000017500000001274313217200022017773 00000000000000# pthread_rwlock_rdlock.m4 serial 1 dnl Copyright (C) 2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Inspired by dnl https://github.com/linux-test-project/ltp/blob/master/testcases/open_posix_testsuite/conformance/interfaces/pthread_rwlock_rdlock/2-2.c dnl by Intel Corporation. dnl Test whether in a situation where dnl - an rwlock is taken by a reader and has a writer waiting, dnl - an additional reader requests the lock, dnl - the waiting writer and the requesting reader threads have the same dnl priority, dnl the requesting reader thread gets blocked, so that at some point the dnl waiting writer can acquire the lock. dnl Without such a guarantee, when there a N readers and each of the readers dnl spends more than 1/Nth of the time with the lock held, there is a high dnl probability that the waiting writer will not get the lock in a given finite dnl time, a phenomenon called "writer starvation". dnl Without such a guarantee, applications have a hard time avoiding writer dnl starvation. dnl dnl POSIX:2008 makes this requirement only for implementations that support TPS dnl (Thread Priority Scheduling) and only for the scheduling policies SCHED_FIFO dnl and SCHED_RR, see dnl http://pubs.opengroup.org/onlinepubs/9699919799/functions/pthread_rwlock_rdlock.html dnl but test verifies the guarantee regardless of TPS and regardless of dnl scheduling policy. AC_DEFUN([gl_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER], [ AC_REQUIRE([gl_THREADLIB_EARLY]) AC_CACHE_CHECK([whether pthread_rwlock_rdlock prefers a writer to a reader], [gl_cv_pthread_rwlock_rdlock_prefer_writer], [save_LIBS="$LIBS" LIBS="$LIBS $LIBMULTITHREAD" AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #define SUCCEED() exit (0) #define FAILURE() exit (1) #define UNEXPECTED(n) (exit (10 + (n))) /* The main thread creates the waiting writer and the requesting reader threads in the default way; this guarantees that they have the same priority. We can reuse the main thread as first reader thread. */ static pthread_rwlock_t lock; static pthread_t reader1; static pthread_t writer; static pthread_t reader2; static pthread_t timer; /* Used to pass control from writer to reader2 and from reader2 to timer, as in a relay race. Passing control from one running thread to another running thread is most likely faster than to create the second thread. */ static pthread_mutex_t baton; static void * timer_func (void *ignored) { /* Step 13 (can be before or after step 12): The timer thread takes the baton, then waits a moment to make sure it can tell whether the second reader thread is blocked at step 12. */ if (pthread_mutex_lock (&baton)) UNEXPECTED (13); usleep (100000); /* By the time we get here, it's clear that the second reader thread is blocked at step 12. This is the desired behaviour. */ SUCCEED (); } static void * reader2_func (void *ignored) { int err; /* Step 8 (can be before or after step 7): The second reader thread takes the baton, then waits a moment to make sure the writer thread has reached step 7. */ if (pthread_mutex_lock (&baton)) UNEXPECTED (8); usleep (100000); /* Step 9: The second reader thread requests the lock. */ err = pthread_rwlock_tryrdlock (&lock); if (err == 0) FAILURE (); else if (err != EBUSY) UNEXPECTED (9); /* Step 10: Launch a timer, to test whether the next call blocks. */ if (pthread_create (&timer, NULL, timer_func, NULL)) UNEXPECTED (10); /* Step 11: Release the baton. */ if (pthread_mutex_unlock (&baton)) UNEXPECTED (11); /* Step 12: The second reader thread requests the lock. */ err = pthread_rwlock_rdlock (&lock); if (err == 0) FAILURE (); else UNEXPECTED (12); } static void * writer_func (void *ignored) { /* Step 4: Take the baton, so that the second reader thread does not go ahead too early. */ if (pthread_mutex_lock (&baton)) UNEXPECTED (4); /* Step 5: Create the second reader thread. */ if (pthread_create (&reader2, NULL, reader2_func, NULL)) UNEXPECTED (5); /* Step 6: Release the baton. */ if (pthread_mutex_unlock (&baton)) UNEXPECTED (6); /* Step 7: The writer thread requests the lock. */ if (pthread_rwlock_wrlock (&lock)) UNEXPECTED (7); return NULL; } int main () { reader1 = pthread_self (); /* Step 1: The main thread initializes the lock and the baton. */ if (pthread_rwlock_init (&lock, NULL)) UNEXPECTED (1); if (pthread_mutex_init (&baton, NULL)) UNEXPECTED (1); /* Step 2: The main thread acquires the lock as a reader. */ if (pthread_rwlock_rdlock (&lock)) UNEXPECTED (2); /* Step 3: Create the writer thread. */ if (pthread_create (&writer, NULL, writer_func, NULL)) UNEXPECTED (3); /* Job done. Go to sleep. */ for (;;) { sleep (1); } } ]])], [gl_cv_pthread_rwlock_rdlock_prefer_writer=yes], [gl_cv_pthread_rwlock_rdlock_prefer_writer=no], [gl_cv_pthread_rwlock_rdlock_prefer_writer="guessing yes"]) LIBS="$save_LIBS" ]) case "$gl_cv_pthread_rwlock_rdlock_prefer_writer" in *yes) AC_DEFINE([HAVE_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER], [1], [Define if the 'pthread_rwlock_rdlock' function prefers a writer to a reader.]) ;; esac ]) gnuastro-0.5/bootstrapped/m4/printf.m40000644000175000017500000017437713217200022014743 00000000000000# printf.m4 serial 57 dnl Copyright (C) 2003, 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Test whether the *printf family of functions supports the 'j', 'z', 't', dnl 'L' size specifiers. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_sizes_c99. AC_DEFUN([gl_PRINTF_SIZES_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_AC_HEADER_STDINT_H]) AC_REQUIRE([gl_AC_HEADER_INTTYPES_H]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports size specifiers as in C99], [gl_cv_func_printf_sizes_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #if HAVE_STDINT_H_WITH_UINTMAX # include #endif #if HAVE_INTTYPES_H_WITH_UINTMAX # include #endif static char buf[100]; int main () { int result = 0; #if HAVE_STDINT_H_WITH_UINTMAX || HAVE_INTTYPES_H_WITH_UINTMAX buf[0] = '\0'; if (sprintf (buf, "%ju %d", (uintmax_t) 12345671, 33, 44, 55) < 0 || strcmp (buf, "12345671 33") != 0) result |= 1; #else result |= 1; #endif buf[0] = '\0'; if (sprintf (buf, "%zu %d", (size_t) 12345672, 33, 44, 55) < 0 || strcmp (buf, "12345672 33") != 0) result |= 2; buf[0] = '\0'; if (sprintf (buf, "%tu %d", (ptrdiff_t) 12345673, 33, 44, 55) < 0 || strcmp (buf, "12345673 33") != 0) result |= 4; buf[0] = '\0'; if (sprintf (buf, "%Lg %d", (long double) 1.5, 33, 44, 55) < 0 || strcmp (buf, "1.5 33") != 0) result |= 8; return result; }]])], [gl_cv_func_printf_sizes_c99=yes], [gl_cv_func_printf_sizes_c99=no], [ case "$host_os" in changequote(,)dnl # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_printf_sizes_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_printf_sizes_c99="guessing no";; darwin*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_printf_sizes_c99="guessing no";; openbsd*) gl_cv_func_printf_sizes_c99="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_printf_sizes_c99="guessing no";; netbsd*) gl_cv_func_printf_sizes_c99="guessing yes";; changequote([,])dnl # Guess yes on MSVC, no on mingw. mingw*) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_func_printf_sizes_c99="guessing yes"], [gl_cv_func_printf_sizes_c99="guessing no"]) ;; # If we don't know, assume the worst. *) gl_cv_func_printf_sizes_c99="guessing no";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports 'long double' dnl arguments together with the 'L' size specifier. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_long_double. AC_DEFUN([gl_PRINTF_LONG_DOUBLE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports 'long double' arguments], [gl_cv_func_printf_long_double], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[10000]; int main () { int result = 0; buf[0] = '\0'; if (sprintf (buf, "%Lf %d", 1.75L, 33, 44, 55) < 0 || strcmp (buf, "1.750000 33") != 0) result |= 1; buf[0] = '\0'; if (sprintf (buf, "%Le %d", 1.75L, 33, 44, 55) < 0 || strcmp (buf, "1.750000e+00 33") != 0) result |= 2; buf[0] = '\0'; if (sprintf (buf, "%Lg %d", 1.75L, 33, 44, 55) < 0 || strcmp (buf, "1.75 33") != 0) result |= 4; return result; }]])], [gl_cv_func_printf_long_double=yes], [gl_cv_func_printf_long_double=no], [case "$host_os" in beos*) gl_cv_func_printf_long_double="guessing no";; # Guess yes on MSVC, no on mingw. mingw*) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_func_printf_long_double="guessing yes"], [gl_cv_func_printf_long_double="guessing no"]) ;; *) gl_cv_func_printf_long_double="guessing yes";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports infinite and NaN dnl 'double' arguments and negative zero arguments in the %f, %e, %g dnl directives. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_infinite. AC_DEFUN([gl_PRINTF_INFINITE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports infinite 'double' arguments], [gl_cv_func_printf_infinite], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static int strisnan (const char *string, size_t start_index, size_t end_index) { if (start_index < end_index) { if (string[start_index] == '-') start_index++; if (start_index + 3 <= end_index && memcmp (string + start_index, "nan", 3) == 0) { start_index += 3; if (start_index == end_index || (string[start_index] == '(' && string[end_index - 1] == ')')) return 1; } } return 0; } static int have_minus_zero () { static double plus_zero = 0.0; double minus_zero = - plus_zero; return memcmp (&plus_zero, &minus_zero, sizeof (double)) != 0; } static char buf[10000]; static double zero = 0.0; int main () { int result = 0; if (sprintf (buf, "%f", 1.0 / zero) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%f", -1.0 / zero) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%f", zero / zero) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%e", 1.0 / zero) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 4; if (sprintf (buf, "%e", -1.0 / zero) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 4; if (sprintf (buf, "%e", zero / zero) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 8; if (sprintf (buf, "%g", 1.0 / zero) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 16; if (sprintf (buf, "%g", -1.0 / zero) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 16; if (sprintf (buf, "%g", zero / zero) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 32; /* This test fails on HP-UX 10.20. */ if (have_minus_zero ()) if (sprintf (buf, "%g", - zero) < 0 || strcmp (buf, "-0") != 0) result |= 64; return result; }]])], [gl_cv_func_printf_infinite=yes], [gl_cv_func_printf_infinite=no], [ case "$host_os" in changequote(,)dnl # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on FreeBSD >= 6. freebsd[1-5].*) gl_cv_func_printf_infinite="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_printf_infinite="guessing no";; darwin*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on HP-UX >= 11. hpux[7-9]* | hpux10*) gl_cv_func_printf_infinite="guessing no";; hpux*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_printf_infinite="guessing no";; netbsd*) gl_cv_func_printf_infinite="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_printf_infinite="guessing yes";; changequote([,])dnl # Guess yes on MSVC, no on mingw. mingw*) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_func_printf_infinite="guessing yes"], [gl_cv_func_printf_infinite="guessing no"]) ;; # If we don't know, assume the worst. *) gl_cv_func_printf_infinite="guessing no";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports infinite and NaN dnl 'long double' arguments in the %f, %e, %g directives. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_infinite_long_double. AC_DEFUN([gl_PRINTF_INFINITE_LONG_DOUBLE], [ AC_REQUIRE([gl_PRINTF_LONG_DOUBLE]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_BIGENDIAN]) AC_REQUIRE([gl_LONG_DOUBLE_VS_DOUBLE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl The user can set or unset the variable gl_printf_safe to indicate dnl that he wishes a safe handling of non-IEEE-754 'long double' values. if test -n "$gl_printf_safe"; then AC_DEFINE([CHECK_PRINTF_SAFE], [1], [Define if you wish *printf() functions that have a safe handling of non-IEEE-754 'long double' values.]) fi case "$gl_cv_func_printf_long_double" in *yes) AC_CACHE_CHECK([whether printf supports infinite 'long double' arguments], [gl_cv_func_printf_infinite_long_double], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ ]GL_NOCRASH[ #include #include #include static int strisnan (const char *string, size_t start_index, size_t end_index) { if (start_index < end_index) { if (string[start_index] == '-') start_index++; if (start_index + 3 <= end_index && memcmp (string + start_index, "nan", 3) == 0) { start_index += 3; if (start_index == end_index || (string[start_index] == '(' && string[end_index - 1] == ')')) return 1; } } return 0; } static char buf[10000]; static long double zeroL = 0.0L; int main () { int result = 0; nocrash_init(); if (sprintf (buf, "%Lf", 1.0L / zeroL) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%Lf", -1.0L / zeroL) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%Lf", zeroL / zeroL) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 1; if (sprintf (buf, "%Le", 1.0L / zeroL) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%Le", -1.0L / zeroL) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%Le", zeroL / zeroL) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 1; if (sprintf (buf, "%Lg", 1.0L / zeroL) < 0 || (strcmp (buf, "inf") != 0 && strcmp (buf, "infinity") != 0)) result |= 1; if (sprintf (buf, "%Lg", -1.0L / zeroL) < 0 || (strcmp (buf, "-inf") != 0 && strcmp (buf, "-infinity") != 0)) result |= 1; if (sprintf (buf, "%Lg", zeroL / zeroL) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 1; #if CHECK_PRINTF_SAFE && ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Representation of an 80-bit 'long double' as an initializer for a sequence of 'unsigned int' words. */ # ifdef WORDS_BIGENDIAN # define LDBL80_WORDS(exponent,manthi,mantlo) \ { ((unsigned int) (exponent) << 16) | ((unsigned int) (manthi) >> 16), \ ((unsigned int) (manthi) << 16) | ((unsigned int) (mantlo) >> 16), \ (unsigned int) (mantlo) << 16 \ } # else # define LDBL80_WORDS(exponent,manthi,mantlo) \ { mantlo, manthi, exponent } # endif { /* Quiet NaN. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0xC3333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Le", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Lg", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; } { /* Signalling NaN. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0x83333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Le", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; if (sprintf (buf, "%Lg", x.value) < 0 || !strisnan (buf, 0, strlen (buf))) result |= 2; } { /* Pseudo-NaN. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0x40000001, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 4; if (sprintf (buf, "%Le", x.value) <= 0) result |= 4; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 4; } { /* Pseudo-Infinity. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0xFFFF, 0x00000000, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 8; if (sprintf (buf, "%Le", x.value) <= 0) result |= 8; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 8; } { /* Pseudo-Zero. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0x4004, 0x00000000, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 16; if (sprintf (buf, "%Le", x.value) <= 0) result |= 16; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 16; } { /* Unnormalized number. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0x4000, 0x63333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 32; if (sprintf (buf, "%Le", x.value) <= 0) result |= 32; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 32; } { /* Pseudo-Denormal. */ static union { unsigned int word[4]; long double value; } x = { LDBL80_WORDS (0x0000, 0x83333333, 0x00000000) }; if (sprintf (buf, "%Lf", x.value) <= 0) result |= 64; if (sprintf (buf, "%Le", x.value) <= 0) result |= 64; if (sprintf (buf, "%Lg", x.value) <= 0) result |= 64; } #endif return result; }]])], [gl_cv_func_printf_infinite_long_double=yes], [gl_cv_func_printf_infinite_long_double=no], [case "$host_cpu" in # Guess no on ia64, x86_64, i386. ia64 | x86_64 | i*86) gl_cv_func_printf_infinite_long_double="guessing no";; *) case "$host_os" in changequote(,)dnl # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_infinite_long_double="guessing yes";; # Guess yes on FreeBSD >= 6. freebsd[1-5].*) gl_cv_func_printf_infinite_long_double="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_infinite_long_double="guessing yes";; # Guess yes on HP-UX >= 11. hpux[7-9]* | hpux10*) gl_cv_func_printf_infinite_long_double="guessing no";; hpux*) gl_cv_func_printf_infinite_long_double="guessing yes";; changequote([,])dnl # Guess yes on MSVC, no on mingw. mingw*) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_func_printf_infinite_long_double="guessing yes"], [gl_cv_func_printf_infinite_long_double="guessing no"]) ;; # If we don't know, assume the worst. *) gl_cv_func_printf_infinite_long_double="guessing no";; esac ;; esac ]) ]) ;; *) gl_cv_func_printf_infinite_long_double="irrelevant" ;; esac ]) dnl Test whether the *printf family of functions supports the 'a' and 'A' dnl conversion specifier for hexadecimal output of floating-point numbers. dnl (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_directive_a. AC_DEFUN([gl_PRINTF_DIRECTIVE_A], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'a' and 'A' directives], [gl_cv_func_printf_directive_a], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; static double zero = 0.0; int main () { int result = 0; if (sprintf (buf, "%a %d", 3.1416015625, 33, 44, 55) < 0 || (strcmp (buf, "0x1.922p+1 33") != 0 && strcmp (buf, "0x3.244p+0 33") != 0 && strcmp (buf, "0x6.488p-1 33") != 0 && strcmp (buf, "0xc.91p-2 33") != 0)) result |= 1; if (sprintf (buf, "%A %d", -3.1416015625, 33, 44, 55) < 0 || (strcmp (buf, "-0X1.922P+1 33") != 0 && strcmp (buf, "-0X3.244P+0 33") != 0 && strcmp (buf, "-0X6.488P-1 33") != 0 && strcmp (buf, "-0XC.91P-2 33") != 0)) result |= 2; /* This catches a FreeBSD 6.1 bug: it doesn't round. */ if (sprintf (buf, "%.2a %d", 1.51, 33, 44, 55) < 0 || (strcmp (buf, "0x1.83p+0 33") != 0 && strcmp (buf, "0x3.05p-1 33") != 0 && strcmp (buf, "0x6.0ap-2 33") != 0 && strcmp (buf, "0xc.14p-3 33") != 0)) result |= 4; /* This catches a Mac OS X 10.12.4 (Darwin 16.5) bug: it doesn't round. */ if (sprintf (buf, "%.0a %d", 1.51, 33, 44, 55) < 0 || (strcmp (buf, "0x2p+0 33") != 0 && strcmp (buf, "0x3p-1 33") != 0 && strcmp (buf, "0x6p-2 33") != 0 && strcmp (buf, "0xcp-3 33") != 0)) result |= 4; /* This catches a FreeBSD 6.1 bug. See */ if (sprintf (buf, "%010a %d", 1.0 / zero, 33, 44, 55) < 0 || buf[0] == '0') result |= 8; /* This catches a Mac OS X 10.3.9 (Darwin 7.9) bug. */ if (sprintf (buf, "%.1a", 1.999) < 0 || (strcmp (buf, "0x1.0p+1") != 0 && strcmp (buf, "0x2.0p+0") != 0 && strcmp (buf, "0x4.0p-1") != 0 && strcmp (buf, "0x8.0p-2") != 0)) result |= 16; /* This catches the same Mac OS X 10.3.9 (Darwin 7.9) bug and also a glibc 2.4 bug . */ if (sprintf (buf, "%.1La", 1.999L) < 0 || (strcmp (buf, "0x1.0p+1") != 0 && strcmp (buf, "0x2.0p+0") != 0 && strcmp (buf, "0x4.0p-1") != 0 && strcmp (buf, "0x8.0p-2") != 0)) result |= 32; return result; }]])], [gl_cv_func_printf_directive_a=yes], [gl_cv_func_printf_directive_a=no], [ case "$host_os" in # Guess yes on glibc >= 2.5 systems. *-gnu*) AC_EGREP_CPP([BZ2908], [ #include #ifdef __GNU_LIBRARY__ #if ((__GLIBC__ == 2 && __GLIBC_MINOR__ >= 5) || (__GLIBC__ > 2)) && !defined __UCLIBC__ BZ2908 #endif #endif ], [gl_cv_func_printf_directive_a="guessing yes"], [gl_cv_func_printf_directive_a="guessing no"]) ;; # Guess no on native Windows. mingw*) gl_cv_func_printf_directive_a="guessing no";; # If we don't know, assume the worst. *) gl_cv_func_printf_directive_a="guessing no";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports the %F format dnl directive. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_directive_f. AC_DEFUN([gl_PRINTF_DIRECTIVE_F], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'F' directive], [gl_cv_func_printf_directive_f], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; static double zero = 0.0; int main () { int result = 0; if (sprintf (buf, "%F %d", 1234567.0, 33, 44, 55) < 0 || strcmp (buf, "1234567.000000 33") != 0) result |= 1; if (sprintf (buf, "%F", 1.0 / zero) < 0 || (strcmp (buf, "INF") != 0 && strcmp (buf, "INFINITY") != 0)) result |= 2; /* This catches a Cygwin 1.5.x bug. */ if (sprintf (buf, "%.F", 1234.0) < 0 || strcmp (buf, "1234") != 0) result |= 4; return result; }]])], [gl_cv_func_printf_directive_f=yes], [gl_cv_func_printf_directive_f=no], [ case "$host_os" in changequote(,)dnl # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_directive_f="guessing yes";; # Guess yes on FreeBSD >= 6. freebsd[1-5].*) gl_cv_func_printf_directive_f="guessing no";; freebsd* | kfreebsd*) gl_cv_func_printf_directive_f="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_printf_directive_f="guessing no";; darwin*) gl_cv_func_printf_directive_f="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_directive_f="guessing yes";; solaris*) gl_cv_func_printf_directive_f="guessing no";; changequote([,])dnl # Guess yes on MSVC, no on mingw. mingw*) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_func_printf_directive_f="guessing yes"], [gl_cv_func_printf_directive_f="guessing no"]) ;; # If we don't know, assume the worst. *) gl_cv_func_printf_directive_f="guessing no";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports the %n format dnl directive. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_printf_directive_n. AC_DEFUN([gl_PRINTF_DIRECTIVE_N], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'n' directive], [gl_cv_func_printf_directive_n], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #ifdef _MSC_VER /* See page about "Parameter Validation" on msdn.microsoft.com. */ static void cdecl invalid_parameter_handler (const wchar_t *expression, const wchar_t *function, const wchar_t *file, unsigned int line, uintptr_t dummy) { exit (1); } #endif static char fmtstring[10]; static char buf[100]; int main () { int count = -1; #ifdef _MSC_VER _set_invalid_parameter_handler (invalid_parameter_handler); #endif /* Copy the format string. Some systems (glibc with _FORTIFY_SOURCE=2) support %n in format strings in read-only memory but not in writable memory. */ strcpy (fmtstring, "%d %n"); if (sprintf (buf, fmtstring, 123, &count, 33, 44, 55) < 0 || strcmp (buf, "123 ") != 0 || count != 4) return 1; return 0; }]])], [gl_cv_func_printf_directive_n=yes], [gl_cv_func_printf_directive_n=no], [case "$host_os" in # Guess no on native Windows. mingw*) gl_cv_func_printf_directive_n="guessing no";; *) gl_cv_func_printf_directive_n="guessing yes";; esac ]) ]) ]) dnl Test whether the *printf family of functions supports the %ls format dnl directive and in particular, when a precision is specified, whether dnl the functions stop converting the wide string argument when the number dnl of bytes that have been produced by this conversion equals or exceeds dnl the precision. dnl Result is gl_cv_func_printf_directive_ls. AC_DEFUN([gl_PRINTF_DIRECTIVE_LS], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the 'ls' directive], [gl_cv_func_printf_directive_ls], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include int main () { int result = 0; char buf[100]; /* Test whether %ls works at all. This test fails on OpenBSD 4.0, IRIX 6.5, Solaris 2.6, Haiku, but not on Cygwin 1.5. */ { static const wchar_t wstring[] = { 'a', 'b', 'c', 0 }; buf[0] = '\0'; if (sprintf (buf, "%ls", wstring) < 0 || strcmp (buf, "abc") != 0) result |= 1; } /* This test fails on IRIX 6.5, Solaris 2.6, Cygwin 1.5, Haiku (with an assertion failure inside libc), but not on OpenBSD 4.0. */ { static const wchar_t wstring[] = { 'a', 0 }; buf[0] = '\0'; if (sprintf (buf, "%ls", wstring) < 0 || strcmp (buf, "a") != 0) result |= 2; } /* Test whether precisions in %ls are supported as specified in ISO C 99 section 7.19.6.1: "If a precision is specified, no more than that many bytes are written (including shift sequences, if any), and the array shall contain a null wide character if, to equal the multibyte character sequence length given by the precision, the function would need to access a wide character one past the end of the array." This test fails on Solaris 10. */ { static const wchar_t wstring[] = { 'a', 'b', (wchar_t) 0xfdfdfdfd, 0 }; buf[0] = '\0'; if (sprintf (buf, "%.2ls", wstring) < 0 || strcmp (buf, "ab") != 0) result |= 8; } return result; }]])], [gl_cv_func_printf_directive_ls=yes], [gl_cv_func_printf_directive_ls=no], [ changequote(,)dnl case "$host_os" in openbsd*) gl_cv_func_printf_directive_ls="guessing no";; irix*) gl_cv_func_printf_directive_ls="guessing no";; solaris*) gl_cv_func_printf_directive_ls="guessing no";; cygwin*) gl_cv_func_printf_directive_ls="guessing no";; beos* | haiku*) gl_cv_func_printf_directive_ls="guessing no";; # Guess yes on native Windows. mingw*) gl_cv_func_printf_directive_ls="guessing yes";; *) gl_cv_func_printf_directive_ls="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports POSIX/XSI format dnl strings with positions. (POSIX:2001) dnl Result is gl_cv_func_printf_positions. AC_DEFUN([gl_PRINTF_POSITIONS], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports POSIX/XSI format strings with positions], [gl_cv_func_printf_positions], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* The string "%2$d %1$d", with dollar characters protected from the shell's dollar expansion (possibly an autoconf bug). */ static char format[] = { '%', '2', '$', 'd', ' ', '%', '1', '$', 'd', '\0' }; static char buf[100]; int main () { sprintf (buf, format, 33, 55); return (strcmp (buf, "55 33") != 0); }]])], [gl_cv_func_printf_positions=yes], [gl_cv_func_printf_positions=no], [ changequote(,)dnl case "$host_os" in netbsd[1-3]* | netbsdelf[1-3]* | netbsdaout[1-3]* | netbsdcoff[1-3]*) gl_cv_func_printf_positions="guessing no";; beos*) gl_cv_func_printf_positions="guessing no";; # Guess no on native Windows. mingw* | pw*) gl_cv_func_printf_positions="guessing no";; *) gl_cv_func_printf_positions="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports POSIX/XSI format dnl strings with the ' flag for grouping of decimal digits. (POSIX:2001) dnl Result is gl_cv_func_printf_flag_grouping. AC_DEFUN([gl_PRINTF_FLAG_GROUPING], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the grouping flag], [gl_cv_func_printf_flag_grouping], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; int main () { if (sprintf (buf, "%'d %d", 1234567, 99) < 0 || buf[strlen (buf) - 1] != '9') return 1; return 0; }]])], [gl_cv_func_printf_flag_grouping=yes], [gl_cv_func_printf_flag_grouping=no], [ changequote(,)dnl case "$host_os" in cygwin*) gl_cv_func_printf_flag_grouping="guessing no";; netbsd*) gl_cv_func_printf_flag_grouping="guessing no";; # Guess no on native Windows. mingw* | pw*) gl_cv_func_printf_flag_grouping="guessing no";; *) gl_cv_func_printf_flag_grouping="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports the - flag correctly. dnl (ISO C99.) See dnl dnl Result is gl_cv_func_printf_flag_leftadjust. AC_DEFUN([gl_PRINTF_FLAG_LEFTADJUST], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the left-adjust flag correctly], [gl_cv_func_printf_flag_leftadjust], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; int main () { /* Check that a '-' flag is not annihilated by a negative width. */ if (sprintf (buf, "a%-*sc", -3, "b") < 0 || strcmp (buf, "ab c") != 0) return 1; return 0; }]])], [gl_cv_func_printf_flag_leftadjust=yes], [gl_cv_func_printf_flag_leftadjust=no], [ changequote(,)dnl case "$host_os" in # Guess yes on HP-UX 11. hpux11*) gl_cv_func_printf_flag_leftadjust="guessing yes";; # Guess no on HP-UX 10 and older. hpux*) gl_cv_func_printf_flag_leftadjust="guessing no";; # Guess yes on native Windows. mingw*) gl_cv_func_printf_flag_leftadjust="guessing yes";; # Guess yes otherwise. *) gl_cv_func_printf_flag_leftadjust="guessing yes";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports padding of non-finite dnl values with the 0 flag correctly. (ISO C99 + TC1 + TC2.) See dnl dnl Result is gl_cv_func_printf_flag_zero. AC_DEFUN([gl_PRINTF_FLAG_ZERO], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports the zero flag correctly], [gl_cv_func_printf_flag_zero], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[100]; static double zero = 0.0; int main () { if (sprintf (buf, "%010f", 1.0 / zero, 33, 44, 55) < 0 || (strcmp (buf, " inf") != 0 && strcmp (buf, " infinity") != 0)) return 1; return 0; }]])], [gl_cv_func_printf_flag_zero=yes], [gl_cv_func_printf_flag_zero=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_flag_zero="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_printf_flag_zero="guessing yes";; # Guess no on native Windows. mingw*) gl_cv_func_printf_flag_zero="guessing no";; # If we don't know, assume the worst. *) gl_cv_func_printf_flag_zero="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions supports large precisions. dnl On mingw, precisions larger than 512 are treated like 512, in integer, dnl floating-point or pointer output. On Solaris 10/x86, precisions larger dnl than 510 in floating-point output crash the program. On Solaris 10/SPARC, dnl precisions larger than 510 in floating-point output yield wrong results. dnl On AIX 7.1, precisions larger than 998 in floating-point output yield dnl wrong results. On BeOS, precisions larger than 1044 crash the program. dnl Result is gl_cv_func_printf_precision. AC_DEFUN([gl_PRINTF_PRECISION], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf supports large precisions], [gl_cv_func_printf_precision], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static char buf[5000]; int main () { int result = 0; #ifdef __BEOS__ /* On BeOS, this would crash and show a dialog box. Avoid the crash. */ return 1; #endif if (sprintf (buf, "%.4000d %d", 1, 33, 44) < 4000 + 3) result |= 1; if (sprintf (buf, "%.4000f %d", 1.0, 33, 44) < 4000 + 5) result |= 2; if (sprintf (buf, "%.511f %d", 1.0, 33, 44) < 511 + 5 || buf[0] != '1') result |= 4; if (sprintf (buf, "%.999f %d", 1.0, 33, 44) < 999 + 5 || buf[0] != '1') result |= 4; return result; }]])], [gl_cv_func_printf_precision=yes], [gl_cv_func_printf_precision=no], [ changequote(,)dnl case "$host_os" in # Guess no only on Solaris, native Windows, and BeOS systems. solaris*) gl_cv_func_printf_precision="guessing no" ;; mingw* | pw*) gl_cv_func_printf_precision="guessing no" ;; beos*) gl_cv_func_printf_precision="guessing no" ;; *) gl_cv_func_printf_precision="guessing yes" ;; esac changequote([,])dnl ]) ]) ]) dnl Test whether the *printf family of functions recovers gracefully in case dnl of an out-of-memory condition, or whether it crashes the entire program. dnl Result is gl_cv_func_printf_enomem. AC_DEFUN([gl_PRINTF_ENOMEM], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_MULTIARCH]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether printf survives out-of-memory conditions], [gl_cv_func_printf_enomem], [ gl_cv_func_printf_enomem="guessing no" if test "$cross_compiling" = no; then if test $APPLE_UNIVERSAL_BUILD = 0; then AC_LANG_CONFTEST([AC_LANG_SOURCE([ ]GL_NOCRASH[ changequote(,)dnl #include #include #include #include #include int main() { struct rlimit limit; int ret; nocrash_init (); /* Some printf implementations allocate temporary space with malloc. */ /* On BSD systems, malloc() is limited by RLIMIT_DATA. */ #ifdef RLIMIT_DATA if (getrlimit (RLIMIT_DATA, &limit) < 0) return 77; if (limit.rlim_max == RLIM_INFINITY || limit.rlim_max > 5000000) limit.rlim_max = 5000000; limit.rlim_cur = limit.rlim_max; if (setrlimit (RLIMIT_DATA, &limit) < 0) return 77; #endif /* On Linux systems, malloc() is limited by RLIMIT_AS. */ #ifdef RLIMIT_AS if (getrlimit (RLIMIT_AS, &limit) < 0) return 77; if (limit.rlim_max == RLIM_INFINITY || limit.rlim_max > 5000000) limit.rlim_max = 5000000; limit.rlim_cur = limit.rlim_max; if (setrlimit (RLIMIT_AS, &limit) < 0) return 77; #endif /* Some printf implementations allocate temporary space on the stack. */ #ifdef RLIMIT_STACK if (getrlimit (RLIMIT_STACK, &limit) < 0) return 77; if (limit.rlim_max == RLIM_INFINITY || limit.rlim_max > 5000000) limit.rlim_max = 5000000; limit.rlim_cur = limit.rlim_max; if (setrlimit (RLIMIT_STACK, &limit) < 0) return 77; #endif ret = printf ("%.5000000f", 1.0); return !(ret == 5000002 || (ret < 0 && errno == ENOMEM)); } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then (./conftest 2>&AS_MESSAGE_LOG_FD result=$? _AS_ECHO_LOG([\$? = $result]) if test $result != 0 && test $result != 77; then result=1; fi exit $result ) >/dev/null 2>/dev/null case $? in 0) gl_cv_func_printf_enomem="yes" ;; 77) gl_cv_func_printf_enomem="guessing no" ;; *) gl_cv_func_printf_enomem="no" ;; esac else gl_cv_func_printf_enomem="guessing no" fi rm -fr conftest* else dnl A universal build on Apple Mac OS X platforms. dnl The result would be 'no' in 32-bit mode and 'yes' in 64-bit mode. dnl But we need a configuration result that is valid in both modes. gl_cv_func_printf_enomem="guessing no" fi fi if test "$gl_cv_func_printf_enomem" = "guessing no"; then changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on Solaris. solaris*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on AIX. aix*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on HP-UX/hppa. hpux*) case "$host_cpu" in hppa*) gl_cv_func_printf_enomem="guessing yes";; *) gl_cv_func_printf_enomem="guessing no";; esac ;; # Guess yes on IRIX. irix*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on OSF/1. osf*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_printf_enomem="guessing yes";; # Guess yes on Haiku. haiku*) gl_cv_func_printf_enomem="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_printf_enomem="guessing no";; esac changequote([,])dnl fi ]) ]) dnl Test whether the snprintf function exists. (ISO C99, POSIX:2001) dnl Result is ac_cv_func_snprintf. AC_DEFUN([gl_SNPRINTF_PRESENCE], [ AC_CHECK_FUNCS_ONCE([snprintf]) ]) dnl Test whether the string produced by the snprintf function is always NUL dnl terminated. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_snprintf_truncation_c99. AC_DEFUN([gl_SNPRINTF_TRUNCATION_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf truncates the result as in C99], [gl_cv_func_snprintf_truncation_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char buf[100]; int main () { strcpy (buf, "ABCDEF"); my_snprintf (buf, 3, "%d %d", 4567, 89); if (memcmp (buf, "45\0DEF", 6) != 0) return 1; return 0; }]])], [gl_cv_func_snprintf_truncation_c99=yes], [gl_cv_func_snprintf_truncation_c99=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_truncation_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_truncation_c99="guessing no";; darwin*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_snprintf_truncation_c99="guessing no";; openbsd*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on Solaris >= 2.6. solaris2.[0-5] | solaris2.[0-5].*) gl_cv_func_snprintf_truncation_c99="guessing no";; solaris*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_truncation_c99="guessing no";; aix*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on HP-UX >= 11. hpux[7-9]* | hpux10*) gl_cv_func_snprintf_truncation_c99="guessing no";; hpux*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on IRIX >= 6.5. irix6.5) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on OSF/1 >= 5. osf[3-4]*) gl_cv_func_snprintf_truncation_c99="guessing no";; osf*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_truncation_c99="guessing no";; netbsd*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_truncation_c99="guessing yes";; # Guess no on native Windows. mingw*) gl_cv_func_snprintf_truncation_c99="guessing no";; # If we don't know, assume the worst. *) gl_cv_func_snprintf_truncation_c99="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the return value of the snprintf function is the number dnl of bytes (excluding the terminating NUL) that would have been produced dnl if the buffer had been large enough. (ISO C99, POSIX:2001) dnl For example, this test program fails on IRIX 6.5: dnl --------------------------------------------------------------------- dnl #include dnl int main() dnl { dnl static char buf[8]; dnl int retval = snprintf (buf, 3, "%d", 12345); dnl return retval >= 0 && retval < 3; dnl } dnl --------------------------------------------------------------------- dnl Result is gl_cv_func_snprintf_retval_c99. AC_DEFUN_ONCE([gl_SNPRINTF_RETVAL_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf returns a byte count as in C99], [gl_cv_func_snprintf_retval_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char buf[100]; int main () { strcpy (buf, "ABCDEF"); if (my_snprintf (buf, 3, "%d %d", 4567, 89) != 7) return 1; if (my_snprintf (buf, 0, "%d %d", 4567, 89) != 7) return 2; if (my_snprintf (NULL, 0, "%d %d", 4567, 89) != 7) return 3; return 0; }]])], [gl_cv_func_snprintf_retval_c99=yes], [gl_cv_func_snprintf_retval_c99=no], [case "$host_os" in changequote(,)dnl # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_retval_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_retval_c99="guessing no";; darwin*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on OpenBSD >= 3.9. openbsd[1-2].* | openbsd3.[0-8] | openbsd3.[0-8].*) gl_cv_func_snprintf_retval_c99="guessing no";; openbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on Solaris >= 2.10. solaris2.[1-9][0-9]*) gl_cv_func_printf_sizes_c99="guessing yes";; solaris*) gl_cv_func_printf_sizes_c99="guessing no";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_retval_c99="guessing no";; aix*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_retval_c99="guessing no";; netbsd*) gl_cv_func_snprintf_retval_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_retval_c99="guessing yes";; changequote([,])dnl # Guess yes on MSVC, no on mingw. mingw*) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_func_snprintf_retval_c99="guessing yes"], [gl_cv_func_snprintf_retval_c99="guessing no"]) ;; # If we don't know, assume the worst. *) gl_cv_func_snprintf_retval_c99="guessing no";; esac ]) ]) ]) dnl Test whether the snprintf function supports the %n format directive dnl also in truncated portions of the format string. (ISO C99, POSIX:2001) dnl Result is gl_cv_func_snprintf_directive_n. AC_DEFUN([gl_SNPRINTF_DIRECTIVE_N], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf fully supports the 'n' directive], [gl_cv_func_snprintf_directive_n], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif static char fmtstring[10]; static char buf[100]; int main () { int count = -1; /* Copy the format string. Some systems (glibc with _FORTIFY_SOURCE=2) support %n in format strings in read-only memory but not in writable memory. */ strcpy (fmtstring, "%d %n"); my_snprintf (buf, 4, fmtstring, 12345, &count, 33, 44, 55); if (count != 6) return 1; return 0; }]])], [gl_cv_func_snprintf_directive_n=yes], [gl_cv_func_snprintf_directive_n=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_snprintf_directive_n="guessing no";; freebsd* | kfreebsd*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_snprintf_directive_n="guessing no";; darwin*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on Solaris >= 2.6. solaris2.[0-5] | solaris2.[0-5].*) gl_cv_func_snprintf_directive_n="guessing no";; solaris*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_snprintf_directive_n="guessing no";; aix*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on IRIX >= 6.5. irix6.5) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on OSF/1 >= 5. osf[3-4]*) gl_cv_func_snprintf_directive_n="guessing no";; osf*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_snprintf_directive_n="guessing no";; netbsd*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_snprintf_directive_n="guessing yes";; # Guess no on native Windows. mingw*) gl_cv_func_snprintf_directive_n="guessing no";; # If we don't know, assume the worst. *) gl_cv_func_snprintf_directive_n="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl Test whether the snprintf function, when passed a size = 1, writes any dnl output without bounds in this case, behaving like sprintf. This is the dnl case on Linux libc5. dnl Result is gl_cv_func_snprintf_size1. AC_DEFUN([gl_SNPRINTF_SIZE1], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_SNPRINTF_PRESENCE]) AC_CACHE_CHECK([whether snprintf respects a size of 1], [gl_cv_func_snprintf_size1], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #if HAVE_SNPRINTF # define my_snprintf snprintf #else # include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } #endif int main() { static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; my_snprintf (buf, 1, "%d", 12345); return buf[1] != 'E'; }]])], [gl_cv_func_snprintf_size1=yes], [gl_cv_func_snprintf_size1=no], [case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_func_snprintf_size1="guessing yes" ;; *) gl_cv_func_snprintf_size1="guessing yes" ;; esac ]) ]) ]) dnl Test whether the vsnprintf function, when passed a zero size, produces no dnl output. (ISO C99, POSIX:2001) dnl For example, snprintf nevertheless writes a NUL byte in this case dnl on OSF/1 5.1: dnl --------------------------------------------------------------------- dnl #include dnl int main() dnl { dnl static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; dnl snprintf (buf, 0, "%d", 12345); dnl return buf[0] != 'D'; dnl } dnl --------------------------------------------------------------------- dnl And vsnprintf writes any output without bounds in this case, behaving like dnl vsprintf, on HP-UX 11 and OSF/1 5.1: dnl --------------------------------------------------------------------- dnl #include dnl #include dnl static int my_snprintf (char *buf, int size, const char *format, ...) dnl { dnl va_list args; dnl int ret; dnl va_start (args, format); dnl ret = vsnprintf (buf, size, format, args); dnl va_end (args); dnl return ret; dnl } dnl int main() dnl { dnl static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; dnl my_snprintf (buf, 0, "%d", 12345); dnl return buf[0] != 'D'; dnl } dnl --------------------------------------------------------------------- dnl Result is gl_cv_func_vsnprintf_zerosize_c99. AC_DEFUN([gl_VSNPRINTF_ZEROSIZE_C99], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether vsnprintf respects a zero size as in C99], [gl_cv_func_vsnprintf_zerosize_c99], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include static int my_snprintf (char *buf, int size, const char *format, ...) { va_list args; int ret; va_start (args, format); ret = vsnprintf (buf, size, format, args); va_end (args); return ret; } int main() { static char buf[8] = { 'D', 'E', 'A', 'D', 'B', 'E', 'E', 'F' }; my_snprintf (buf, 0, "%d", 12345); return buf[0] != 'D'; }]])], [gl_cv_func_vsnprintf_zerosize_c99=yes], [gl_cv_func_vsnprintf_zerosize_c99=no], [ changequote(,)dnl case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on FreeBSD >= 5. freebsd[1-4].*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; freebsd* | kfreebsd*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on Mac OS X >= 10.3. darwin[1-6].*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; darwin*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on Cygwin. cygwin*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on Solaris >= 2.6. solaris2.[0-5] | solaris2.[0-5].*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; solaris*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on AIX >= 4. aix[1-3]*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; aix*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on IRIX >= 6.5. irix6.5) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on NetBSD >= 3. netbsd[1-2]* | netbsdelf[1-2]* | netbsdaout[1-2]* | netbsdcoff[1-2]*) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; netbsd*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on BeOS. beos*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # Guess yes on native Windows. mingw* | pw*) gl_cv_func_vsnprintf_zerosize_c99="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_vsnprintf_zerosize_c99="guessing no";; esac changequote([,])dnl ]) ]) ]) dnl The results of these tests on various platforms are: dnl dnl 1 = gl_PRINTF_SIZES_C99 dnl 2 = gl_PRINTF_LONG_DOUBLE dnl 3 = gl_PRINTF_INFINITE dnl 4 = gl_PRINTF_INFINITE_LONG_DOUBLE dnl 5 = gl_PRINTF_DIRECTIVE_A dnl 6 = gl_PRINTF_DIRECTIVE_F dnl 7 = gl_PRINTF_DIRECTIVE_N dnl 8 = gl_PRINTF_DIRECTIVE_LS dnl 9 = gl_PRINTF_POSITIONS dnl 10 = gl_PRINTF_FLAG_GROUPING dnl 11 = gl_PRINTF_FLAG_LEFTADJUST dnl 12 = gl_PRINTF_FLAG_ZERO dnl 13 = gl_PRINTF_PRECISION dnl 14 = gl_PRINTF_ENOMEM dnl 15 = gl_SNPRINTF_PRESENCE dnl 16 = gl_SNPRINTF_TRUNCATION_C99 dnl 17 = gl_SNPRINTF_RETVAL_C99 dnl 18 = gl_SNPRINTF_DIRECTIVE_N dnl 19 = gl_SNPRINTF_SIZE1 dnl 20 = gl_VSNPRINTF_ZEROSIZE_C99 dnl dnl 1 = checking whether printf supports size specifiers as in C99... dnl 2 = checking whether printf supports 'long double' arguments... dnl 3 = checking whether printf supports infinite 'double' arguments... dnl 4 = checking whether printf supports infinite 'long double' arguments... dnl 5 = checking whether printf supports the 'a' and 'A' directives... dnl 6 = checking whether printf supports the 'F' directive... dnl 7 = checking whether printf supports the 'n' directive... dnl 8 = checking whether printf supports the 'ls' directive... dnl 9 = checking whether printf supports POSIX/XSI format strings with positions... dnl 10 = checking whether printf supports the grouping flag... dnl 11 = checking whether printf supports the left-adjust flag correctly... dnl 12 = checking whether printf supports the zero flag correctly... dnl 13 = checking whether printf supports large precisions... dnl 14 = checking whether printf survives out-of-memory conditions... dnl 15 = checking for snprintf... dnl 16 = checking whether snprintf truncates the result as in C99... dnl 17 = checking whether snprintf returns a byte count as in C99... dnl 18 = checking whether snprintf fully supports the 'n' directive... dnl 19 = checking whether snprintf respects a size of 1... dnl 20 = checking whether vsnprintf respects a zero size as in C99... dnl dnl . = yes, # = no. dnl dnl 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 dnl glibc 2.5 . . . . . . . . . . . . . . . . . . . . dnl glibc 2.3.6 . . . . # . . . . . . . . . . . . . . . dnl FreeBSD 5.4, 6.1 . . . . # . . . . . . # . # . . . . . . dnl Mac OS X 10.5.8 . . . # # . . . . . . # . . . . . . . . dnl Mac OS X 10.3.9 . . . . # . . . . . . # . # . . . . . . dnl OpenBSD 3.9, 4.0 . . # # # # . # . # . # . # . . . . . . dnl Cygwin 1.7.0 (2009) . . . # . . . ? . . . . . ? . . . . . . dnl Cygwin 1.5.25 (2008) . . . # # . . # . . . . . # . . . . . . dnl Cygwin 1.5.19 (2006) # . . # # # . # . # . # # # . . . . . . dnl Solaris 11.3 . . . . # . . # . . . . . . . . . . . . dnl Solaris 11.0 . . # # # . . # . . . # . . . . . . . . dnl Solaris 10 . . # # # . . # . . . # # . . . . . . . dnl Solaris 2.6 ... 9 # . # # # # . # . . . # # . . . # . . . dnl Solaris 2.5.1 # . # # # # . # . . . # . . # # # # # # dnl AIX 7.1 . . # # # . . . . . . # # . . . . . . . dnl AIX 5.2 . . # # # . . . . . . # . . . . . . . . dnl AIX 4.3.2, 5.1 # . # # # # . . . . . # . . . . # . . . dnl HP-UX 11.31 . . . . # . . . . . . # . . . . # # . . dnl HP-UX 11.{00,11,23} # . . . # # . . . . . # . . . . # # . # dnl HP-UX 10.20 # . # . # # . ? . . # # . . . . # # ? # dnl IRIX 6.5 # . # # # # . # . . . # . . . . # . . . dnl OSF/1 5.1 # . # # # # . . . . . # . . . . # . . # dnl OSF/1 4.0d # . # # # # . . . . . # . . # # # # # # dnl NetBSD 5.0 . . . # # . . . . . . # . # . . . . . . dnl NetBSD 4.0 . ? ? ? ? ? . ? . ? ? ? ? ? . . . ? ? ? dnl NetBSD 3.0 . . . . # # . ? # # ? # . # . . . . . . dnl Haiku . . . # # # . # . . . . . ? . . ? . . . dnl BeOS # # . # # # . ? # . ? . # ? . . ? . . . dnl old mingw / msvcrt # # # # # # . . # # . # # ? . # # # . . dnl MSVC 9 # # # # # # # . # # . # # ? # # # # . . dnl mingw 2009-2011 . # . # . . . . # # . . . ? . . . . . . dnl mingw-w64 2011 # # # # # # . . # # . # # ? . # # # . . gnuastro-0.5/bootstrapped/m4/pipe.m40000644000175000017500000000066013217200022014355 00000000000000# pipe.m4 serial 2 dnl Copyright (C) 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_PIPE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([pipe]) if test $ac_cv_func_pipe != yes; then HAVE_PIPE=0 fi ]) gnuastro-0.5/bootstrapped/m4/perror.m40000644000175000017500000000476613217200022014744 00000000000000# perror.m4 serial 7 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_PERROR], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) AC_REQUIRE([gl_HEADER_ERRNO_H]) AC_REQUIRE([gl_FUNC_STRERROR_R]) AC_REQUIRE([gl_FUNC_STRERROR_0]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl We intentionally do not check for the broader REPLACE_STRERROR_R, dnl since on glibc systems, strerror_r is replaced only for signature dnl issues, and perror is just fine. Rather, we only want to dnl replace perror if strerror_r was replaced for a content fix. if test "$ERRNO_H:$REPLACE_STRERROR_0" != :0; then dnl The system's perror() cannot know about the new errno values we add dnl to , or any fix for strerror(0). Replace it. REPLACE_PERROR=1 fi case ${gl_cv_func_strerror_r_works-unset} in unset|*yes) AC_CACHE_CHECK([whether perror matches strerror], [gl_cv_func_perror_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include #include ]], [[char *str = strerror (-1); if (!getenv("CONFTEST_OUTPUT")) return 0; if (!str) str = ""; puts (str); errno = -1; perror (""); return 0; ]])], [if CONFTEST_OUTPUT=1 ./conftest$EXEEXT >conftest.txt1 2>conftest.txt2 \ && cmp conftest.txt1 conftest.txt2 >/dev/null; then gl_cv_func_perror_works=yes else gl_cv_func_perror_works=no fi rm -rf conftest.txt1 conftest.txt2], [gl_cv_func_perror_works=no], [case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_func_perror_works="guessing yes" ;; # Otherwise guess no. *) gl_cv_func_perror_works="guessing no" ;; esac ]) ]) case "$gl_cv_func_perror_works" in *yes) ;; *) REPLACE_PERROR=1 ;; esac ;; *) dnl The system's perror() probably inherits the bugs in the dnl system's strerror_r(). Replace it. REPLACE_PERROR=1 ;; esac ]) gnuastro-0.5/bootstrapped/m4/pathmax.m40000644000175000017500000000220413217200022015056 00000000000000# pathmax.m4 serial 10 dnl Copyright (C) 2002-2003, 2005-2006, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_PATHMAX], [ dnl Prerequisites of lib/pathmax.h. AC_CHECK_HEADERS_ONCE([sys/param.h]) ]) # Expands to a piece of C program that defines PATH_MAX in the same way as # "pathmax.h" will do. AC_DEFUN([gl_PATHMAX_SNIPPET], [[ /* Arrange to define PATH_MAX, like "pathmax.h" does. */ #if HAVE_UNISTD_H # include #endif #include #if defined HAVE_SYS_PARAM_H && !defined PATH_MAX && !defined MAXPATHLEN # include #endif #if !defined PATH_MAX && defined MAXPATHLEN # define PATH_MAX MAXPATHLEN #endif #ifdef __hpux # undef PATH_MAX # define PATH_MAX 1024 #endif #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ # undef PATH_MAX # define PATH_MAX 260 #endif ]]) # Prerequisites of gl_PATHMAX_SNIPPET. AC_DEFUN([gl_PATHMAX_SNIPPET_PREREQ], [ AC_CHECK_HEADERS_ONCE([unistd.h sys/param.h]) ]) gnuastro-0.5/bootstrapped/m4/open.m40000644000175000017500000000523713217200022014366 00000000000000# open.m4 serial 15 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_OPEN], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_PREPROC_O_CLOEXEC]) case "$host_os" in mingw* | pw*) REPLACE_OPEN=1 ;; *) dnl open("foo/") should not create a file when the file name has a dnl trailing slash. FreeBSD only has the problem on symlinks. AC_CHECK_FUNCS_ONCE([lstat]) if test "$gl_cv_macro_O_CLOEXEC" != yes; then REPLACE_OPEN=1 fi AC_CACHE_CHECK([whether open recognizes a trailing slash], [gl_cv_func_open_slash], [# Assume that if we have lstat, we can also check symlinks. if test $ac_cv_func_lstat = yes; then touch conftest.tmp ln -s conftest.tmp conftest.lnk fi AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #if HAVE_UNISTD_H # include #endif int main () { int result = 0; #if HAVE_LSTAT if (open ("conftest.lnk/", O_RDONLY) != -1) result |= 1; #endif if (open ("conftest.sl/", O_CREAT, 0600) >= 0) result |= 2; return result; }]])], [gl_cv_func_open_slash=yes], [gl_cv_func_open_slash=no], [ changequote(,)dnl case "$host_os" in freebsd* | aix* | hpux* | solaris2.[0-9] | solaris2.[0-9].*) gl_cv_func_open_slash="guessing no" ;; *) gl_cv_func_open_slash="guessing yes" ;; esac changequote([,])dnl ]) rm -f conftest.sl conftest.tmp conftest.lnk ]) case "$gl_cv_func_open_slash" in *no) AC_DEFINE([OPEN_TRAILING_SLASH_BUG], [1], [Define to 1 if open() fails to recognize a trailing slash.]) REPLACE_OPEN=1 ;; esac ;; esac dnl Replace open() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ if test $REPLACE_OPEN = 0; then gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then REPLACE_OPEN=1 fi fi ]) dnl Replace open() for supporting the gnulib-defined O_NONBLOCK flag. m4_ifdef([gl_NONBLOCKING_IO], [ if test $REPLACE_OPEN = 0; then gl_NONBLOCKING_IO if test $gl_cv_have_open_O_NONBLOCK != yes; then REPLACE_OPEN=1 fi fi ]) ]) # Prerequisites of lib/open.c. AC_DEFUN([gl_PREREQ_OPEN], [ AC_REQUIRE([gl_PROMOTED_TYPE_MODE_T]) : ]) gnuastro-0.5/bootstrapped/m4/open-cloexec.m40000644000175000017500000000131613217200022016000 00000000000000# Test whether O_CLOEXEC is defined. dnl Copyright 2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_PREPROC_O_CLOEXEC], [ AC_CACHE_CHECK([for O_CLOEXEC], [gl_cv_macro_O_CLOEXEC], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include #ifndef O_CLOEXEC choke me; #endif ]], [[return O_CLOEXEC;]])], [gl_cv_macro_O_CLOEXEC=yes], [gl_cv_macro_O_CLOEXEC=no])]) ]) gnuastro-0.5/bootstrapped/m4/off_t.m40000644000175000017500000000100613217200022014510 00000000000000# off_t.m4 serial 1 dnl Copyright (C) 2012-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Check whether to override the 'off_t' type. dnl Set WINDOWS_64_BIT_OFF_T. AC_DEFUN([gl_TYPE_OFF_T], [ m4_ifdef([gl_LARGEFILE], [ AC_REQUIRE([gl_LARGEFILE]) ], [ WINDOWS_64_BIT_OFF_T=0 ]) AC_SUBST([WINDOWS_64_BIT_OFF_T]) ]) gnuastro-0.5/bootstrapped/m4/nproc.m40000644000175000017500000000347013217200022014543 00000000000000# nproc.m4 serial 5 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_NPROC], [ gl_PREREQ_NPROC ]) # Prerequisites of lib/nproc.c. AC_DEFUN([gl_PREREQ_NPROC], [ dnl Persuade glibc to declare CPU_SETSIZE, CPU_ISSET etc. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS([sys/pstat.h sys/sysmp.h sys/param.h],,, [AC_INCLUDES_DEFAULT]) dnl requires on OpenBSD 4.0. AC_CHECK_HEADERS([sys/sysctl.h],,, [AC_INCLUDES_DEFAULT #if HAVE_SYS_PARAM_H # include #endif ]) AC_CHECK_FUNCS([sched_getaffinity sched_getaffinity_np \ pstat_getdynamic sysmp sysctl]) dnl Test whether sched_getaffinity has the expected declaration. dnl glibc 2.3.[0-2]: dnl int sched_getaffinity (pid_t, unsigned int, unsigned long int *); dnl glibc 2.3.3: dnl int sched_getaffinity (pid_t, cpu_set_t *); dnl glibc >= 2.3.4: dnl int sched_getaffinity (pid_t, size_t, cpu_set_t *); if test $ac_cv_func_sched_getaffinity = yes; then AC_CACHE_CHECK([for glibc compatible sched_getaffinity], [gl_cv_func_sched_getaffinity3], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include ]], [[sched_getaffinity (0, 0, (cpu_set_t *) 0);]])], [gl_cv_func_sched_getaffinity3=yes], [gl_cv_func_sched_getaffinity3=no]) ]) if test $gl_cv_func_sched_getaffinity3 = yes; then AC_DEFINE([HAVE_SCHED_GETAFFINITY_LIKE_GLIBC], [1], [Define to 1 if sched_getaffinity has a glibc compatible declaration.]) fi fi ]) gnuastro-0.5/bootstrapped/m4/nocrash.m40000644000175000017500000001060213217200022015052 00000000000000# nocrash.m4 serial 4 dnl Copyright (C) 2005, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Based on libsigsegv, from Bruno Haible and Paolo Bonzini. AC_PREREQ([2.13]) dnl Expands to some code for use in .c programs that will cause the configure dnl test to exit instead of crashing. This is useful to avoid triggering dnl action from a background debugger and to avoid core dumps. dnl Usage: ... dnl ]GL_NOCRASH[ dnl ... dnl int main() { nocrash_init(); ... } AC_DEFUN([GL_NOCRASH],[[ #include #if defined __MACH__ && defined __APPLE__ /* Avoid a crash on Mac OS X. */ #include #include #include #include #include #include /* The exception port on which our thread listens. */ static mach_port_t our_exception_port; /* The main function of the thread listening for exceptions of type EXC_BAD_ACCESS. */ static void * mach_exception_thread (void *arg) { /* Buffer for a message to be received. */ struct { mach_msg_header_t head; mach_msg_body_t msgh_body; char data[1024]; } msg; mach_msg_return_t retval; /* Wait for a message on the exception port. */ retval = mach_msg (&msg.head, MACH_RCV_MSG | MACH_RCV_LARGE, 0, sizeof (msg), our_exception_port, MACH_MSG_TIMEOUT_NONE, MACH_PORT_NULL); if (retval != MACH_MSG_SUCCESS) abort (); exit (1); } static void nocrash_init (void) { mach_port_t self = mach_task_self (); /* Allocate a port on which the thread shall listen for exceptions. */ if (mach_port_allocate (self, MACH_PORT_RIGHT_RECEIVE, &our_exception_port) == KERN_SUCCESS) { /* See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/mach_port_insert_right.html. */ if (mach_port_insert_right (self, our_exception_port, our_exception_port, MACH_MSG_TYPE_MAKE_SEND) == KERN_SUCCESS) { /* The exceptions we want to catch. Only EXC_BAD_ACCESS is interesting for us. */ exception_mask_t mask = EXC_MASK_BAD_ACCESS; /* Create the thread listening on the exception port. */ pthread_attr_t attr; pthread_t thread; if (pthread_attr_init (&attr) == 0 && pthread_attr_setdetachstate (&attr, PTHREAD_CREATE_DETACHED) == 0 && pthread_create (&thread, &attr, mach_exception_thread, NULL) == 0) { pthread_attr_destroy (&attr); /* Replace the exception port info for these exceptions with our own. Note that we replace the exception port for the entire task, not only for a particular thread. This has the effect that when our exception port gets the message, the thread specific exception port has already been asked, and we don't need to bother about it. See http://web.mit.edu/darwin/src/modules/xnu/osfmk/man/task_set_exception_ports.html. */ task_set_exception_ports (self, mask, our_exception_port, EXCEPTION_DEFAULT, MACHINE_THREAD_STATE); } } } } #elif (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* Avoid a crash on native Windows. */ #define WIN32_LEAN_AND_MEAN #include #include static LONG WINAPI exception_filter (EXCEPTION_POINTERS *ExceptionInfo) { switch (ExceptionInfo->ExceptionRecord->ExceptionCode) { case EXCEPTION_ACCESS_VIOLATION: case EXCEPTION_IN_PAGE_ERROR: case EXCEPTION_STACK_OVERFLOW: case EXCEPTION_GUARD_PAGE: case EXCEPTION_PRIV_INSTRUCTION: case EXCEPTION_ILLEGAL_INSTRUCTION: case EXCEPTION_DATATYPE_MISALIGNMENT: case EXCEPTION_ARRAY_BOUNDS_EXCEEDED: case EXCEPTION_NONCONTINUABLE_EXCEPTION: exit (1); } return EXCEPTION_CONTINUE_SEARCH; } static void nocrash_init (void) { SetUnhandledExceptionFilter ((LPTOP_LEVEL_EXCEPTION_FILTER) exception_filter); } #else /* Avoid a crash on POSIX systems. */ #include #include /* A POSIX signal handler. */ static void exception_handler (int sig) { _exit (1); } static void nocrash_init (void) { #ifdef SIGSEGV signal (SIGSEGV, exception_handler); #endif #ifdef SIGBUS signal (SIGBUS, exception_handler); #endif } #endif ]]) gnuastro-0.5/bootstrapped/m4/nl_langinfo.m40000644000175000017500000000352413217200022015710 00000000000000# nl_langinfo.m4 serial 5 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_NL_LANGINFO], [ AC_REQUIRE([gl_LANGINFO_H_DEFAULTS]) AC_REQUIRE([gl_LANGINFO_H]) AC_CHECK_FUNCS_ONCE([nl_langinfo]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles if test $ac_cv_func_nl_langinfo = yes; then # On Irix 6.5, YESEXPR is defined, but nl_langinfo(YESEXPR) is broken. AC_CACHE_CHECK([whether YESEXPR works], [gl_cv_func_nl_langinfo_yesexpr_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[return !*nl_langinfo(YESEXPR); ]])], [gl_cv_func_nl_langinfo_yesexpr_works=yes], [gl_cv_func_nl_langinfo_yesexpr_works=no], [ case "$host_os" in # Guess no on irix systems. irix*) gl_cv_func_nl_langinfo_yesexpr_works="guessing no";; # Guess yes elsewhere. *) gl_cv_func_nl_langinfo_yesexpr_works="guessing yes";; esac ]) ]) case $gl_cv_func_nl_langinfo_yesexpr_works in *yes) FUNC_NL_LANGINFO_YESEXPR_WORKS=1 ;; *) FUNC_NL_LANGINFO_YESEXPR_WORKS=0 ;; esac AC_DEFINE_UNQUOTED([FUNC_NL_LANGINFO_YESEXPR_WORKS], [$FUNC_NL_LANGINFO_YESEXPR_WORKS], [Define to 1 if nl_langinfo (YESEXPR) returns a non-empty string.]) if test $HAVE_LANGINFO_CODESET = 1 && test $HAVE_LANGINFO_ERA = 1 \ && test $FUNC_NL_LANGINFO_YESEXPR_WORKS = 1; then : else REPLACE_NL_LANGINFO=1 AC_DEFINE([REPLACE_NL_LANGINFO], [1], [Define if nl_langinfo exists but is overridden by gnulib.]) fi else HAVE_NL_LANGINFO=0 fi ]) gnuastro-0.5/bootstrapped/m4/netinet_in_h.m40000644000175000017500000000207513217200022016065 00000000000000# netinet_in_h.m4 serial 5 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_HEADER_NETINET_IN], [ AC_CACHE_CHECK([whether is self-contained], [gl_cv_header_netinet_in_h_selfcontained], [ AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[]])], [gl_cv_header_netinet_in_h_selfcontained=yes], [gl_cv_header_netinet_in_h_selfcontained=no]) ]) if test $gl_cv_header_netinet_in_h_selfcontained = yes; then NETINET_IN_H='' else NETINET_IN_H='netinet/in.h' AC_CHECK_HEADERS([netinet/in.h]) gl_CHECK_NEXT_HEADERS([netinet/in.h]) if test $ac_cv_header_netinet_in_h = yes; then HAVE_NETINET_IN_H=1 else HAVE_NETINET_IN_H=0 fi AC_SUBST([HAVE_NETINET_IN_H]) fi AC_SUBST([NETINET_IN_H]) AM_CONDITIONAL([GL_GENERATE_NETINET_IN_H], [test -n "$NETINET_IN_H"]) ]) gnuastro-0.5/bootstrapped/m4/nanosleep.m40000644000175000017500000001127113217200022015404 00000000000000# serial 37 dnl From Jim Meyering. dnl Check for the nanosleep function. dnl If not found, use the supplied replacement. dnl # Copyright (C) 1999-2001, 2003-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_NANOSLEEP], [ AC_REQUIRE([gl_HEADER_TIME_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl Persuade glibc and Solaris to declare nanosleep. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS_ONCE([sys/time.h]) AC_REQUIRE([gl_FUNC_SELECT]) nanosleep_save_libs=$LIBS # Solaris 2.5.1 needs -lposix4 to get the nanosleep function. # Solaris 7 prefers the library name -lrt to the obsolescent name -lposix4. LIB_NANOSLEEP= AC_SUBST([LIB_NANOSLEEP]) AC_SEARCH_LIBS([nanosleep], [rt posix4], [test "$ac_cv_search_nanosleep" = "none required" || LIB_NANOSLEEP=$ac_cv_search_nanosleep]) if test "x$ac_cv_search_nanosleep" != xno; then dnl The system has a nanosleep function. AC_REQUIRE([gl_MULTIARCH]) if test $APPLE_UNIVERSAL_BUILD = 1; then # A universal build on Apple Mac OS X platforms. # The test result would be 'no (mishandles large arguments)' in 64-bit # mode but 'yes' in 32-bit mode. But we need a configuration result that # is valid in both modes. gl_cv_func_nanosleep='no (mishandles large arguments)' fi AC_CACHE_CHECK([for working nanosleep], [gl_cv_func_nanosleep], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #if HAVE_SYS_TIME_H #include #endif #include #include #define TYPE_SIGNED(t) (! ((t) 0 < (t) -1)) #define TYPE_MAXIMUM(t) \ ((t) (! TYPE_SIGNED (t) \ ? (t) -1 \ : ((((t) 1 << (sizeof (t) * CHAR_BIT - 2)) - 1) * 2 + 1))) static void check_for_SIGALRM (int sig) { if (sig != SIGALRM) _exit (1); } int main () { static struct timespec ts_sleep; static struct timespec ts_remaining; static struct sigaction act; /* Test for major problems first. */ if (! nanosleep) return 2; act.sa_handler = check_for_SIGALRM; sigemptyset (&act.sa_mask); sigaction (SIGALRM, &act, NULL); ts_sleep.tv_sec = 0; ts_sleep.tv_nsec = 1; alarm (1); if (nanosleep (&ts_sleep, NULL) != 0) return 3; /* Test for a minor problem: the handling of large arguments. */ ts_sleep.tv_sec = TYPE_MAXIMUM (time_t); ts_sleep.tv_nsec = 999999999; alarm (1); if (nanosleep (&ts_sleep, &ts_remaining) != -1) return 4; if (errno != EINTR) return 5; if (ts_remaining.tv_sec <= TYPE_MAXIMUM (time_t) - 10) return 6; return 0; }]])], [gl_cv_func_nanosleep=yes], [case $? in dnl ( 4|5|6) gl_cv_func_nanosleep='no (mishandles large arguments)';; dnl ( *) gl_cv_func_nanosleep=no;; esac], [case "$host_os" in dnl (( linux*) # Guess it halfway works when the kernel is Linux. gl_cv_func_nanosleep='guessing no (mishandles large arguments)' ;; mingw*) # Guess no on native Windows. gl_cv_func_nanosleep='guessing no' ;; *) # If we don't know, assume the worst. gl_cv_func_nanosleep='guessing no' ;; esac ]) ]) case "$gl_cv_func_nanosleep" in *yes) REPLACE_NANOSLEEP=0 ;; *) REPLACE_NANOSLEEP=1 case "$gl_cv_func_nanosleep" in *"mishandles large arguments"*) AC_DEFINE([HAVE_BUG_BIG_NANOSLEEP], [1], [Define to 1 if nanosleep mishandles large arguments.]) ;; *) # The replacement uses select(). Add $LIBSOCKET to $LIB_NANOSLEEP. for ac_lib in $LIBSOCKET; do case " $LIB_NANOSLEEP " in *" $ac_lib "*) ;; *) LIB_NANOSLEEP="$LIB_NANOSLEEP $ac_lib";; esac done ;; esac ;; esac else HAVE_NANOSLEEP=0 fi LIBS=$nanosleep_save_libs ]) # Prerequisites of lib/nanosleep.c. AC_DEFUN([gl_PREREQ_NANOSLEEP], [ AC_CHECK_HEADERS_ONCE([sys/select.h]) gl_PREREQ_SIG_HANDLER_H ]) gnuastro-0.5/bootstrapped/m4/multiarch.m40000644000175000017500000000367413217200022015420 00000000000000# multiarch.m4 serial 7 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Determine whether the compiler is or may be producing universal binaries. # # On Mac OS X 10.5 and later systems, the user can create libraries and # executables that work on multiple system types--known as "fat" or # "universal" binaries--by specifying multiple '-arch' options to the # compiler but only a single '-arch' option to the preprocessor. Like # this: # # ./configure CC="gcc -arch i386 -arch x86_64 -arch ppc -arch ppc64" \ # CXX="g++ -arch i386 -arch x86_64 -arch ppc -arch ppc64" \ # CPP="gcc -E" CXXCPP="g++ -E" # # Detect this situation and set APPLE_UNIVERSAL_BUILD accordingly. AC_DEFUN_ONCE([gl_MULTIARCH], [ dnl Code similar to autoconf-2.63 AC_C_BIGENDIAN. gl_cv_c_multiarch=no AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#ifndef __APPLE_CC__ not a universal capable compiler #endif typedef int dummy; ]])], [ dnl Check for potential -arch flags. It is not universal unless dnl there are at least two -arch flags with different values. arch= prev= for word in ${CC} ${CFLAGS} ${CPPFLAGS} ${LDFLAGS}; do if test -n "$prev"; then case $word in i?86 | x86_64 | ppc | ppc64) if test -z "$arch" || test "$arch" = "$word"; then arch="$word" else gl_cv_c_multiarch=yes fi ;; esac prev= else if test "x$word" = "x-arch"; then prev=arch fi fi done ]) if test $gl_cv_c_multiarch = yes; then APPLE_UNIVERSAL_BUILD=1 else APPLE_UNIVERSAL_BUILD=0 fi AC_SUBST([APPLE_UNIVERSAL_BUILD]) ]) gnuastro-0.5/bootstrapped/m4/msvc-nothrow.m40000644000175000017500000000053013217200022016062 00000000000000# msvc-nothrow.m4 serial 1 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MSVC_NOTHROW], [ AC_REQUIRE([gl_MSVC_INVAL]) ]) gnuastro-0.5/bootstrapped/m4/msvc-inval.m40000644000175000017500000000133413217200022015476 00000000000000# msvc-inval.m4 serial 1 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MSVC_INVAL], [ AC_CHECK_FUNCS_ONCE([_set_invalid_parameter_handler]) if test $ac_cv_func__set_invalid_parameter_handler = yes; then HAVE_MSVC_INVALID_PARAMETER_HANDLER=1 AC_DEFINE([HAVE_MSVC_INVALID_PARAMETER_HANDLER], [1], [Define to 1 on MSVC platforms that have the "invalid parameter handler" concept.]) else HAVE_MSVC_INVALID_PARAMETER_HANDLER=0 fi AC_SUBST([HAVE_MSVC_INVALID_PARAMETER_HANDLER]) ]) gnuastro-0.5/bootstrapped/m4/mode_t.m40000644000175000017500000000234213217200022014666 00000000000000# mode_t.m4 serial 2 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # For using mode_t, it's sufficient to use AC_TYPE_MODE_T and # include . # Define PROMOTED_MODE_T to the type that is the result of "default argument # promotion" (ISO C 6.5.2.2.(6)) of the type mode_t. AC_DEFUN([gl_PROMOTED_TYPE_MODE_T], [ AC_REQUIRE([AC_TYPE_MODE_T]) AC_CACHE_CHECK([for promoted mode_t type], [gl_cv_promoted_mode_t], [ dnl Assume mode_t promotes to 'int' if and only if it is smaller than 'int', dnl and to itself otherwise. This assumption is not guaranteed by the ISO C dnl standard, but we don't know of any real-world counterexamples. AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[#include ]], [[typedef int array[2 * (sizeof (mode_t) < sizeof (int)) - 1];]])], [gl_cv_promoted_mode_t='int'], [gl_cv_promoted_mode_t='mode_t']) ]) AC_DEFINE_UNQUOTED([PROMOTED_MODE_T], [$gl_cv_promoted_mode_t], [Define to the type that is the result of default argument promotions of type mode_t.]) ]) gnuastro-0.5/bootstrapped/m4/mmap-anon.m40000644000175000017500000000373313217200022015307 00000000000000# mmap-anon.m4 serial 10 dnl Copyright (C) 2005, 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Detect how mmap can be used to create anonymous (not file-backed) memory # mappings. # - On Linux, AIX, OSF/1, Solaris, Cygwin, Interix, Haiku, both MAP_ANONYMOUS # and MAP_ANON exist and have the same value. # - On HP-UX, only MAP_ANONYMOUS exists. # - On Mac OS X, FreeBSD, NetBSD, OpenBSD, only MAP_ANON exists. # - On IRIX, neither exists, and a file descriptor opened to /dev/zero must be # used. AC_DEFUN([gl_FUNC_MMAP_ANON], [ dnl Persuade glibc to define MAP_ANONYMOUS. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) # Check for mmap(). Don't use AC_FUNC_MMAP, because it checks too much: it # fails on HP-UX 11, because MAP_FIXED mappings do not work. But this is # irrelevant for anonymous mappings. AC_CHECK_FUNC([mmap], [gl_have_mmap=yes], [gl_have_mmap=no]) # Try to allow MAP_ANONYMOUS. gl_have_mmap_anonymous=no if test $gl_have_mmap = yes; then AC_MSG_CHECKING([for MAP_ANONYMOUS]) AC_EGREP_CPP([I cannot identify this map], [ #include #ifdef MAP_ANONYMOUS I cannot identify this map #endif ], [gl_have_mmap_anonymous=yes]) if test $gl_have_mmap_anonymous != yes; then AC_EGREP_CPP([I cannot identify this map], [ #include #ifdef MAP_ANON I cannot identify this map #endif ], [AC_DEFINE([MAP_ANONYMOUS], [MAP_ANON], [Define to a substitute value for mmap()'s MAP_ANONYMOUS flag.]) gl_have_mmap_anonymous=yes]) fi AC_MSG_RESULT([$gl_have_mmap_anonymous]) if test $gl_have_mmap_anonymous = yes; then AC_DEFINE([HAVE_MAP_ANONYMOUS], [1], [Define to 1 if mmap()'s MAP_ANONYMOUS flag is available after including config.h and .]) fi fi ]) gnuastro-0.5/bootstrapped/m4/minmax.m40000644000175000017500000000245513217200022014715 00000000000000# minmax.m4 serial 4 dnl Copyright (C) 2005, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_PREREQ([2.53]) AC_DEFUN([gl_MINMAX], [ AC_REQUIRE([gl_PREREQ_MINMAX]) ]) # Prerequisites of lib/minmax.h. AC_DEFUN([gl_PREREQ_MINMAX], [ gl_MINMAX_IN_HEADER([limits.h]) gl_MINMAX_IN_HEADER([sys/param.h]) ]) dnl gl_MINMAX_IN_HEADER(HEADER) dnl The parameter has to be a literal header name; it cannot be macro, dnl nor a shell variable. (Because autoheader collects only AC_DEFINE dnl invocations with a literal macro name.) AC_DEFUN([gl_MINMAX_IN_HEADER], [ m4_pushdef([header], AS_TR_SH([$1])) m4_pushdef([HEADER], AS_TR_CPP([$1])) AC_CACHE_CHECK([whether <$1> defines MIN and MAX], [gl_cv_minmax_in_]header, [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include <$1> int x = MIN (42, 17);]], [[]])], [gl_cv_minmax_in_]header[=yes], [gl_cv_minmax_in_]header[=no])]) if test $gl_cv_minmax_in_[]header = yes; then AC_DEFINE([HAVE_MINMAX_IN_]HEADER, 1, [Define to 1 if <$1> defines the MIN and MAX macros.]) fi m4_popdef([HEADER]) m4_popdef([header]) ]) gnuastro-0.5/bootstrapped/m4/mempcpy.m40000644000175000017500000000134613217200022015074 00000000000000# mempcpy.m4 serial 11 dnl Copyright (C) 2003-2004, 2006-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MEMPCPY], [ dnl Persuade glibc to declare mempcpy(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) dnl The mempcpy() declaration in lib/string.in.h uses 'restrict'. AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) AC_CHECK_FUNCS([mempcpy]) if test $ac_cv_func_mempcpy = no; then HAVE_MEMPCPY=0 fi ]) # Prerequisites of lib/mempcpy.c. AC_DEFUN([gl_PREREQ_MEMPCPY], [ : ]) gnuastro-0.5/bootstrapped/m4/memchr.m40000644000175000017500000000602213217200022014671 00000000000000# memchr.m4 serial 13 dnl Copyright (C) 2002-2004, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_FUNC_MEMCHR], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) AC_REQUIRE([gl_HEADER_STRING_H_DEFAULTS]) m4_ifdef([gl_FUNC_MEMCHR_OBSOLETE], [ dnl These days, we assume memchr is present. But if support for old dnl platforms is desired: AC_CHECK_FUNCS_ONCE([memchr]) if test $ac_cv_func_memchr = no; then HAVE_MEMCHR=0 fi ]) if test $HAVE_MEMCHR = 1; then # Detect platform-specific bugs in some versions of glibc: # memchr should not dereference anything with length 0 # https://bugzilla.redhat.com/show_bug.cgi?id=499689 # memchr should not dereference overestimated length after a match # https://bugs.debian.org/cgi-bin/bugreport.cgi?bug=521737 # https://sourceware.org/bugzilla/show_bug.cgi?id=10162 # Assume that memchr works on platforms that lack mprotect. AC_CACHE_CHECK([whether memchr works], [gl_cv_func_memchr_works], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ #include #if HAVE_SYS_MMAN_H # include # include # include # include # ifndef MAP_FILE # define MAP_FILE 0 # endif #endif ]], [[ int result = 0; char *fence = NULL; #if HAVE_SYS_MMAN_H && HAVE_MPROTECT # if HAVE_MAP_ANONYMOUS const int flags = MAP_ANONYMOUS | MAP_PRIVATE; const int fd = -1; # else /* !HAVE_MAP_ANONYMOUS */ const int flags = MAP_FILE | MAP_PRIVATE; int fd = open ("/dev/zero", O_RDONLY, 0666); if (fd >= 0) # endif { int pagesize = getpagesize (); char *two_pages = (char *) mmap (NULL, 2 * pagesize, PROT_READ | PROT_WRITE, flags, fd, 0); if (two_pages != (char *)(-1) && mprotect (two_pages + pagesize, pagesize, PROT_NONE) == 0) fence = two_pages + pagesize; } #endif if (fence) { if (memchr (fence, 0, 0)) result |= 1; strcpy (fence - 9, "12345678"); if (memchr (fence - 9, 0, 79) != fence - 1) result |= 2; if (memchr (fence - 1, 0, 3) != fence - 1) result |= 4; } return result; ]])], [gl_cv_func_memchr_works=yes], [gl_cv_func_memchr_works=no], [case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_func_memchr_works="guessing yes" ;; # Be pessimistic for now. *) gl_cv_func_memchr_works="guessing no" ;; esac ]) ]) case "$gl_cv_func_memchr_works" in *yes) ;; *) REPLACE_MEMCHR=1 ;; esac fi ]) # Prerequisites of lib/memchr.c. AC_DEFUN([gl_PREREQ_MEMCHR], [ AC_CHECK_HEADERS([bp-sym.h]) ]) gnuastro-0.5/bootstrapped/m4/mbtowc.m40000644000175000017500000000071413217200022014713 00000000000000# mbtowc.m4 serial 2 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MBTOWC], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) if false; then REPLACE_MBTOWC=1 fi ]) # Prerequisites of lib/mbtowc.c. AC_DEFUN([gl_PREREQ_MBTOWC], [ : ]) gnuastro-0.5/bootstrapped/m4/mbstate_t.m40000644000175000017500000000256713217200022015412 00000000000000# mbstate_t.m4 serial 13 dnl Copyright (C) 2000-2002, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # From Paul Eggert. # BeOS 5 has but does not define mbstate_t, # so you can't declare an object of that type. # Check for this incompatibility with Standard C. # AC_TYPE_MBSTATE_T # ----------------- AC_DEFUN([AC_TYPE_MBSTATE_T], [ AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) dnl for HP-UX 11.11 AC_CACHE_CHECK([for mbstate_t], [ac_cv_type_mbstate_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [AC_INCLUDES_DEFAULT[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]], [[mbstate_t x; return sizeof x;]])], [ac_cv_type_mbstate_t=yes], [ac_cv_type_mbstate_t=no])]) if test $ac_cv_type_mbstate_t = yes; then AC_DEFINE([HAVE_MBSTATE_T], [1], [Define to 1 if declares mbstate_t.]) else AC_DEFINE([mbstate_t], [int], [Define to a type if does not define.]) fi ]) gnuastro-0.5/bootstrapped/m4/mbsinit.m40000644000175000017500000000276313217200022015073 00000000000000# mbsinit.m4 serial 8 dnl Copyright (C) 2008, 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MBSINIT], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) gl_MBSTATE_T_BROKEN AC_CHECK_FUNCS_ONCE([mbsinit]) if test $ac_cv_func_mbsinit = no; then HAVE_MBSINIT=0 AC_CHECK_DECLS([mbsinit],,, [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_mbsinit = yes; then dnl On Minix 3.1.8, the system's declares mbsinit() although dnl it does not have the function. Avoid a collision with gnulib's dnl replacement. REPLACE_MBSINIT=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBSINIT=1 else dnl On mingw, mbsinit() always returns 1, which is inappropriate for dnl states produced by mbrtowc() for an incomplete multibyte character dnl in multibyte locales. case "$host_os" in mingw*) REPLACE_MBSINIT=1 ;; esac fi fi ]) # Prerequisites of lib/mbsinit.c. AC_DEFUN([gl_PREREQ_MBSINIT], [ : ]) gnuastro-0.5/bootstrapped/m4/mbrtowc.m40000644000175000017500000004776513217200022015116 00000000000000# mbrtowc.m4 serial 29 -*- coding: utf-8 -*- dnl Copyright (C) 2001-2002, 2004-2005, 2008-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_MBRTOWC], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) gl_MBSTATE_T_BROKEN AC_CHECK_FUNCS_ONCE([mbrtowc]) if test $ac_cv_func_mbrtowc = no; then HAVE_MBRTOWC=0 AC_CHECK_DECLS([mbrtowc],,, [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]]) if test $ac_cv_have_decl_mbrtowc = yes; then dnl On Minix 3.1.8, the system's declares mbrtowc() although dnl it does not have the function. Avoid a collision with gnulib's dnl replacement. REPLACE_MBRTOWC=1 fi else if test $REPLACE_MBSTATE_T = 1; then REPLACE_MBRTOWC=1 else gl_MBRTOWC_NULL_ARG1 gl_MBRTOWC_NULL_ARG2 gl_MBRTOWC_RETVAL gl_MBRTOWC_NUL_RETVAL gl_MBRTOWC_EMPTY_INPUT gl_MBRTOWC_C_LOCALE case "$gl_cv_func_mbrtowc_null_arg1" in *yes) ;; *) AC_DEFINE([MBRTOWC_NULL_ARG1_BUG], [1], [Define if the mbrtowc function has the NULL pwc argument bug.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_null_arg2" in *yes) ;; *) AC_DEFINE([MBRTOWC_NULL_ARG2_BUG], [1], [Define if the mbrtowc function has the NULL string argument bug.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_retval" in *yes) ;; *) AC_DEFINE([MBRTOWC_RETVAL_BUG], [1], [Define if the mbrtowc function returns a wrong return value.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_nul_retval" in *yes) ;; *) AC_DEFINE([MBRTOWC_NUL_RETVAL_BUG], [1], [Define if the mbrtowc function does not return 0 for a NUL character.]) REPLACE_MBRTOWC=1 ;; esac case "$gl_cv_func_mbrtowc_empty_input" in *yes) ;; *) AC_DEFINE([MBRTOWC_EMPTY_INPUT_BUG], [1], [Define if the mbrtowc function does not return (size_t) -2 for empty input.]) REPLACE_MBRTOWC=1 ;; esac case $gl_cv_C_locale_sans_EILSEQ in *yes) ;; *) AC_DEFINE([C_LOCALE_MAYBE_EILSEQ], [1], [Define to 1 if the C locale may have encoding errors.]) REPLACE_MBRTOWC=1 ;; esac fi fi ]) dnl Test whether mbsinit() and mbrtowc() need to be overridden in a way that dnl redefines the semantics of the given mbstate_t type. dnl Result is REPLACE_MBSTATE_T. dnl When this is set to 1, we replace both mbsinit() and mbrtowc(), in order to dnl avoid inconsistencies. AC_DEFUN([gl_MBSTATE_T_BROKEN], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) AC_REQUIRE([AC_TYPE_MBSTATE_T]) AC_CHECK_FUNCS_ONCE([mbsinit]) AC_CHECK_FUNCS_ONCE([mbrtowc]) if test $ac_cv_func_mbsinit = yes && test $ac_cv_func_mbrtowc = yes; then gl_MBRTOWC_INCOMPLETE_STATE gl_MBRTOWC_SANITYCHECK REPLACE_MBSTATE_T=0 case "$gl_cv_func_mbrtowc_incomplete_state" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac case "$gl_cv_func_mbrtowc_sanitycheck" in *yes) ;; *) REPLACE_MBSTATE_T=1 ;; esac else REPLACE_MBSTATE_T=1 fi ]) dnl Test whether mbrtowc puts the state into non-initial state when parsing an dnl incomplete multibyte character. dnl Result is gl_cv_func_mbrtowc_incomplete_state. AC_DEFUN([gl_MBRTOWC_INCOMPLETE_STATE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_JA]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc handles incomplete characters], [gl_cv_func_mbrtowc_incomplete_state], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on AIX and OSF/1. aix* | osf*) gl_cv_func_mbrtowc_incomplete_state="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_incomplete_state="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_JA != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { const char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) if (mbsinit (&state)) return 2; } return 0; }]])], [gl_cv_func_mbrtowc_incomplete_state=yes], [gl_cv_func_mbrtowc_incomplete_state=no], [:]) fi ]) ]) dnl Test whether mbrtowc works not worse than mbtowc. dnl Result is gl_cv_func_mbrtowc_sanitycheck. AC_DEFUN([gl_MBRTOWC_SANITYCHECK], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_ZH_CN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc works as well as mbtowc], [gl_cv_func_mbrtowc_sanitycheck], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris 8. solaris2.8) gl_cv_func_mbrtowc_sanitycheck="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_sanitycheck="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_ZH_CN != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8: mbrtowc returns 2, and sets wc to 0x00F0. mbtowc returns 4 (correct) and sets wc to 0x5EDC. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { char input[] = "B\250\271\201\060\211\070er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 6, &state) != 4 && mbtowc (&wc, input + 3, 6) == 4) return 2; } return 0; }]])], [gl_cv_func_mbrtowc_sanitycheck=yes], [gl_cv_func_mbrtowc_sanitycheck=no], [:]) fi ]) ]) dnl Test whether mbrtowc supports a NULL pwc argument correctly. dnl Result is gl_cv_func_mbrtowc_null_arg1. AC_DEFUN([gl_MBRTOWC_NULL_ARG1], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc handles a NULL pwc argument], [gl_cv_func_mbrtowc_null_arg1], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris. solaris*) gl_cv_func_mbrtowc_null_arg1="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg1="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR_UTF8 != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "\303\237er"; mbstate_t state; wchar_t wc; size_t ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; ret = mbrtowc (&wc, input, 5, &state); if (ret != 2) result |= 1; if (!mbsinit (&state)) result |= 2; memset (&state, '\0', sizeof (mbstate_t)); ret = mbrtowc (NULL, input, 5, &state); if (ret != 2) /* Solaris 7 fails here: ret is -1. */ result |= 4; if (!mbsinit (&state)) result |= 8; } return result; }]])], [gl_cv_func_mbrtowc_null_arg1=yes], [gl_cv_func_mbrtowc_null_arg1=no], [:]) fi ]) ]) dnl Test whether mbrtowc supports a NULL string argument correctly. dnl Result is gl_cv_func_mbrtowc_null_arg2. AC_DEFUN([gl_MBRTOWC_NULL_ARG2], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc handles a NULL string argument], [gl_cv_func_mbrtowc_null_arg2], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on OSF/1. osf*) gl_cv_func_mbrtowc_null_arg2="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_null_arg2="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR_UTF8 != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { mbstate_t state; wchar_t wc; int ret; memset (&state, '\0', sizeof (mbstate_t)); wc = (wchar_t) 0xBADFACE; mbrtowc (&wc, NULL, 5, &state); /* Check that wc was not modified. */ if (wc != (wchar_t) 0xBADFACE) return 2; } return 0; }]])], [gl_cv_func_mbrtowc_null_arg2=yes], [gl_cv_func_mbrtowc_null_arg2=no], [:]) fi ]) ]) dnl Test whether mbrtowc, when parsing the end of a multibyte character, dnl correctly returns the number of bytes that were needed to complete the dnl character (not the total number of bytes of the multibyte character). dnl Result is gl_cv_func_mbrtowc_retval. AC_DEFUN([gl_MBRTOWC_RETVAL], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR_UTF8]) AC_REQUIRE([gt_LOCALE_JA]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CACHE_CHECK([whether mbrtowc has a correct return value], [gl_cv_func_mbrtowc_retval], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on HP-UX, Solaris, native Windows. hpux* | solaris* | mingw*) gl_cv_func_mbrtowc_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_retval="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR_UTF8 != none || test $LOCALE_JA != none \ || { case "$host_os" in mingw*) true;; *) false;; esac; }; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { int result = 0; int found_some_locale = 0; /* This fails on Solaris. */ if (setlocale (LC_ALL, "$LOCALE_FR_UTF8") != NULL) { char input[] = "B\303\274\303\237er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 1) result |= 1; } found_some_locale = 1; } /* This fails on HP-UX 11.11. */ if (setlocale (LC_ALL, "$LOCALE_JA") != NULL) { char input[] = "B\217\253\344\217\251\316er"; /* "Büßer" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 1, 1, &state) == (size_t)(-2)) { input[1] = '\0'; if (mbrtowc (&wc, input + 2, 5, &state) != 2) result |= 2; } found_some_locale = 1; } /* This fails on native Windows. */ if (setlocale (LC_ALL, "Japanese_Japan.932") != NULL) { char input[] = "<\223\372\226\173\214\352>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 4; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_Taiwan.950") != NULL) { char input[] = "<\244\351\245\273\273\171>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 8; } found_some_locale = 1; } if (setlocale (LC_ALL, "Chinese_China.936") != NULL) { char input[] = "<\310\325\261\276\325\132>"; /* "<日本語>" */ mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, input + 3, 1, &state) == (size_t)(-2)) { input[3] = '\0'; if (mbrtowc (&wc, input + 4, 4, &state) != 1) result |= 16; } found_some_locale = 1; } return (found_some_locale ? result : 77); }]])], [gl_cv_func_mbrtowc_retval=yes], [if test $? != 77; then gl_cv_func_mbrtowc_retval=no fi ], [:]) fi ]) ]) dnl Test whether mbrtowc, when parsing a NUL character, correctly returns 0. dnl Result is gl_cv_func_mbrtowc_nul_retval. AC_DEFUN([gl_MBRTOWC_NUL_RETVAL], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_ZH_CN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc returns 0 when parsing a NUL character], [gl_cv_func_mbrtowc_nul_retval], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on Solaris 8 and 9. solaris2.[89]) gl_cv_func_mbrtowc_nul_retval="guessing no" ;; # Guess yes otherwise. *) gl_cv_func_mbrtowc_nul_retval="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_ZH_CN != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { /* This fails on Solaris 8 and 9. */ if (setlocale (LC_ALL, "$LOCALE_ZH_CN") != NULL) { mbstate_t state; wchar_t wc; memset (&state, '\0', sizeof (mbstate_t)); if (mbrtowc (&wc, "", 1, &state) != 0) return 2; } return 0; }]])], [gl_cv_func_mbrtowc_nul_retval=yes], [gl_cv_func_mbrtowc_nul_retval=no], [:]) fi ]) ]) dnl Test whether mbrtowc returns the correct value on empty input. AC_DEFUN([gl_MBRTOWC_EMPTY_INPUT], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether mbrtowc works on empty input], [gl_cv_func_mbrtowc_empty_input], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on AIX and glibc systems. aix* | *-gnu*) gl_cv_func_mbrtowc_empty_input="guessing no" ;; # Guess yes on native Windows. mingw*) gl_cv_func_mbrtowc_empty_input="guessing yes" ;; *) gl_cv_func_mbrtowc_empty_input="guessing yes" ;; esac changequote([,])dnl AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include static wchar_t wc; static mbstate_t mbs; int main (void) { return mbrtowc (&wc, "", 0, &mbs) != (size_t) -2; }]])], [gl_cv_func_mbrtowc_empty_input=yes], [gl_cv_func_mbrtowc_empty_input=no], [:]) ]) ]) dnl Test whether mbrtowc reports encoding errors in the C locale. dnl Although POSIX was never intended to allow this, the GNU C Library dnl and other implementations do it. See: dnl https://sourceware.org/bugzilla/show_bug.cgi?id=19932 AC_DEFUN([gl_MBRTOWC_C_LOCALE], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether the C locale is free of encoding errors], [gl_cv_C_locale_sans_EILSEQ], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. gl_cv_C_locale_sans_EILSEQ="guessing no" AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include ]], [[ int i; char *locale = setlocale (LC_ALL, "C"); if (! locale) return 2; for (i = CHAR_MIN; i <= CHAR_MAX; i++) { char c = i; wchar_t wc; mbstate_t mbs = { 0, }; size_t ss = mbrtowc (&wc, &c, 1, &mbs); if (1 < ss) return 3; } return 0; ]])], [gl_cv_C_locale_sans_EILSEQ=yes], [gl_cv_C_locale_sans_EILSEQ=no], [case "$host_os" in # Guess yes on native Windows. mingw*) gl_cv_C_locale_sans_EILSEQ="guessing yes" ;; esac ]) ]) ]) # Prerequisites of lib/mbrtowc.c. AC_DEFUN([gl_PREREQ_MBRTOWC], [ : ]) dnl From Paul Eggert dnl This is an override of an autoconf macro. AC_DEFUN([AC_FUNC_MBRTOWC], [ dnl Same as AC_FUNC_MBRTOWC in autoconf-2.60. AC_CACHE_CHECK([whether mbrtowc and mbstate_t are properly declared], [gl_cv_func_mbrtowc], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[/* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include ]], [[wchar_t wc; char const s[] = ""; size_t n = 1; mbstate_t state; return ! (sizeof state && (mbrtowc) (&wc, s, n, &state));]])], [gl_cv_func_mbrtowc=yes], [gl_cv_func_mbrtowc=no])]) if test $gl_cv_func_mbrtowc = yes; then AC_DEFINE([HAVE_MBRTOWC], [1], [Define to 1 if mbrtowc and mbstate_t are properly declared.]) fi ]) gnuastro-0.5/bootstrapped/m4/mbiter.m40000644000175000017500000000064213217200022014702 00000000000000# mbiter.m4 serial 7 dnl Copyright (C) 2005, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl autoconf tests required for use of mbiter.h dnl From Bruno Haible. AC_DEFUN([gl_MBITER], [ AC_REQUIRE([AC_TYPE_MBSTATE_T]) : ]) gnuastro-0.5/bootstrapped/m4/mbchar.m40000644000175000017500000000065313217200022014656 00000000000000# mbchar.m4 serial 9 dnl Copyright (C) 2005-2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl autoconf tests required for use of mbchar.m4 dnl From Bruno Haible. AC_DEFUN([gl_MBCHAR], [ AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) ]) gnuastro-0.5/bootstrapped/m4/math_h.m40000644000175000017500000004345413217200022014670 00000000000000# math_h.m4 serial 116 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MATH_H], [ AC_REQUIRE([gl_MATH_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([math.h]) AC_CACHE_CHECK([whether NAN macro works], [gl_cv_header_math_nan_works], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[@%:@include ]], [[/* Solaris 10 has a broken definition of NAN. Other platforms fail to provide NAN, or provide it only in C99 mode; this test only needs to fail when NAN is provided but wrong. */ float f = 1.0f; #ifdef NAN f = NAN; #endif return f == 0;]])], [gl_cv_header_math_nan_works=yes], [gl_cv_header_math_nan_works=no])]) if test $gl_cv_header_math_nan_works = no; then REPLACE_NAN=1 fi AC_CACHE_CHECK([whether HUGE_VAL works], [gl_cv_header_math_huge_val_works], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[@%:@include ]], [[/* Solaris 10 has a broken definition of HUGE_VAL. */ double d = HUGE_VAL; return d == 0;]])], [gl_cv_header_math_huge_val_works=yes], [gl_cv_header_math_huge_val_works=no])]) if test $gl_cv_header_math_huge_val_works = no; then REPLACE_HUGE_VAL=1 fi dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [acosf acosl asinf asinl atanf atanl cbrt cbrtf cbrtl ceilf ceill copysign copysignf copysignl cosf cosl coshf expf expl exp2 exp2f exp2l expm1 expm1f expm1l fabsf fabsl floorf floorl fma fmaf fmal fmod fmodf fmodl frexpf frexpl hypotf hypotl ilogb ilogbf ilogbl ldexpf ldexpl log logf logl log10 log10f log10l log1p log1pf log1pl log2 log2f log2l logb logbf logbl modf modff modfl powf remainder remainderf remainderl rint rintf rintl round roundf roundl sinf sinl sinhf sqrtf sqrtl tanf tanl tanhf trunc truncf truncl]) ]) AC_DEFUN([gl_MATH_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_MATH_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_MATH_H_DEFAULTS], [ GNULIB_ACOSF=0; AC_SUBST([GNULIB_ACOSF]) GNULIB_ACOSL=0; AC_SUBST([GNULIB_ACOSL]) GNULIB_ASINF=0; AC_SUBST([GNULIB_ASINF]) GNULIB_ASINL=0; AC_SUBST([GNULIB_ASINL]) GNULIB_ATANF=0; AC_SUBST([GNULIB_ATANF]) GNULIB_ATANL=0; AC_SUBST([GNULIB_ATANL]) GNULIB_ATAN2F=0; AC_SUBST([GNULIB_ATAN2F]) GNULIB_CBRT=0; AC_SUBST([GNULIB_CBRT]) GNULIB_CBRTF=0; AC_SUBST([GNULIB_CBRTF]) GNULIB_CBRTL=0; AC_SUBST([GNULIB_CBRTL]) GNULIB_CEIL=0; AC_SUBST([GNULIB_CEIL]) GNULIB_CEILF=0; AC_SUBST([GNULIB_CEILF]) GNULIB_CEILL=0; AC_SUBST([GNULIB_CEILL]) GNULIB_COPYSIGN=0; AC_SUBST([GNULIB_COPYSIGN]) GNULIB_COPYSIGNF=0; AC_SUBST([GNULIB_COPYSIGNF]) GNULIB_COPYSIGNL=0; AC_SUBST([GNULIB_COPYSIGNL]) GNULIB_COSF=0; AC_SUBST([GNULIB_COSF]) GNULIB_COSL=0; AC_SUBST([GNULIB_COSL]) GNULIB_COSHF=0; AC_SUBST([GNULIB_COSHF]) GNULIB_EXPF=0; AC_SUBST([GNULIB_EXPF]) GNULIB_EXPL=0; AC_SUBST([GNULIB_EXPL]) GNULIB_EXP2=0; AC_SUBST([GNULIB_EXP2]) GNULIB_EXP2F=0; AC_SUBST([GNULIB_EXP2F]) GNULIB_EXP2L=0; AC_SUBST([GNULIB_EXP2L]) GNULIB_EXPM1=0; AC_SUBST([GNULIB_EXPM1]) GNULIB_EXPM1F=0; AC_SUBST([GNULIB_EXPM1F]) GNULIB_EXPM1L=0; AC_SUBST([GNULIB_EXPM1L]) GNULIB_FABSF=0; AC_SUBST([GNULIB_FABSF]) GNULIB_FABSL=0; AC_SUBST([GNULIB_FABSL]) GNULIB_FLOOR=0; AC_SUBST([GNULIB_FLOOR]) GNULIB_FLOORF=0; AC_SUBST([GNULIB_FLOORF]) GNULIB_FLOORL=0; AC_SUBST([GNULIB_FLOORL]) GNULIB_FMA=0; AC_SUBST([GNULIB_FMA]) GNULIB_FMAF=0; AC_SUBST([GNULIB_FMAF]) GNULIB_FMAL=0; AC_SUBST([GNULIB_FMAL]) GNULIB_FMOD=0; AC_SUBST([GNULIB_FMOD]) GNULIB_FMODF=0; AC_SUBST([GNULIB_FMODF]) GNULIB_FMODL=0; AC_SUBST([GNULIB_FMODL]) GNULIB_FREXPF=0; AC_SUBST([GNULIB_FREXPF]) GNULIB_FREXP=0; AC_SUBST([GNULIB_FREXP]) GNULIB_FREXPL=0; AC_SUBST([GNULIB_FREXPL]) GNULIB_HYPOT=0; AC_SUBST([GNULIB_HYPOT]) GNULIB_HYPOTF=0; AC_SUBST([GNULIB_HYPOTF]) GNULIB_HYPOTL=0; AC_SUBST([GNULIB_HYPOTL]) GNULIB_ILOGB=0; AC_SUBST([GNULIB_ILOGB]) GNULIB_ILOGBF=0; AC_SUBST([GNULIB_ILOGBF]) GNULIB_ILOGBL=0; AC_SUBST([GNULIB_ILOGBL]) GNULIB_ISFINITE=0; AC_SUBST([GNULIB_ISFINITE]) GNULIB_ISINF=0; AC_SUBST([GNULIB_ISINF]) GNULIB_ISNAN=0; AC_SUBST([GNULIB_ISNAN]) GNULIB_ISNANF=0; AC_SUBST([GNULIB_ISNANF]) GNULIB_ISNAND=0; AC_SUBST([GNULIB_ISNAND]) GNULIB_ISNANL=0; AC_SUBST([GNULIB_ISNANL]) GNULIB_LDEXPF=0; AC_SUBST([GNULIB_LDEXPF]) GNULIB_LDEXPL=0; AC_SUBST([GNULIB_LDEXPL]) GNULIB_LOG=0; AC_SUBST([GNULIB_LOG]) GNULIB_LOGF=0; AC_SUBST([GNULIB_LOGF]) GNULIB_LOGL=0; AC_SUBST([GNULIB_LOGL]) GNULIB_LOG10=0; AC_SUBST([GNULIB_LOG10]) GNULIB_LOG10F=0; AC_SUBST([GNULIB_LOG10F]) GNULIB_LOG10L=0; AC_SUBST([GNULIB_LOG10L]) GNULIB_LOG1P=0; AC_SUBST([GNULIB_LOG1P]) GNULIB_LOG1PF=0; AC_SUBST([GNULIB_LOG1PF]) GNULIB_LOG1PL=0; AC_SUBST([GNULIB_LOG1PL]) GNULIB_LOG2=0; AC_SUBST([GNULIB_LOG2]) GNULIB_LOG2F=0; AC_SUBST([GNULIB_LOG2F]) GNULIB_LOG2L=0; AC_SUBST([GNULIB_LOG2L]) GNULIB_LOGB=0; AC_SUBST([GNULIB_LOGB]) GNULIB_LOGBF=0; AC_SUBST([GNULIB_LOGBF]) GNULIB_LOGBL=0; AC_SUBST([GNULIB_LOGBL]) GNULIB_MODF=0; AC_SUBST([GNULIB_MODF]) GNULIB_MODFF=0; AC_SUBST([GNULIB_MODFF]) GNULIB_MODFL=0; AC_SUBST([GNULIB_MODFL]) GNULIB_POWF=0; AC_SUBST([GNULIB_POWF]) GNULIB_REMAINDER=0; AC_SUBST([GNULIB_REMAINDER]) GNULIB_REMAINDERF=0; AC_SUBST([GNULIB_REMAINDERF]) GNULIB_REMAINDERL=0; AC_SUBST([GNULIB_REMAINDERL]) GNULIB_RINT=0; AC_SUBST([GNULIB_RINT]) GNULIB_RINTF=0; AC_SUBST([GNULIB_RINTF]) GNULIB_RINTL=0; AC_SUBST([GNULIB_RINTL]) GNULIB_ROUND=0; AC_SUBST([GNULIB_ROUND]) GNULIB_ROUNDF=0; AC_SUBST([GNULIB_ROUNDF]) GNULIB_ROUNDL=0; AC_SUBST([GNULIB_ROUNDL]) GNULIB_SIGNBIT=0; AC_SUBST([GNULIB_SIGNBIT]) GNULIB_SINF=0; AC_SUBST([GNULIB_SINF]) GNULIB_SINL=0; AC_SUBST([GNULIB_SINL]) GNULIB_SINHF=0; AC_SUBST([GNULIB_SINHF]) GNULIB_SQRTF=0; AC_SUBST([GNULIB_SQRTF]) GNULIB_SQRTL=0; AC_SUBST([GNULIB_SQRTL]) GNULIB_TANF=0; AC_SUBST([GNULIB_TANF]) GNULIB_TANL=0; AC_SUBST([GNULIB_TANL]) GNULIB_TANHF=0; AC_SUBST([GNULIB_TANHF]) GNULIB_TRUNC=0; AC_SUBST([GNULIB_TRUNC]) GNULIB_TRUNCF=0; AC_SUBST([GNULIB_TRUNCF]) GNULIB_TRUNCL=0; AC_SUBST([GNULIB_TRUNCL]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_ACOSF=1; AC_SUBST([HAVE_ACOSF]) HAVE_ACOSL=1; AC_SUBST([HAVE_ACOSL]) HAVE_ASINF=1; AC_SUBST([HAVE_ASINF]) HAVE_ASINL=1; AC_SUBST([HAVE_ASINL]) HAVE_ATANF=1; AC_SUBST([HAVE_ATANF]) HAVE_ATANL=1; AC_SUBST([HAVE_ATANL]) HAVE_ATAN2F=1; AC_SUBST([HAVE_ATAN2F]) HAVE_CBRT=1; AC_SUBST([HAVE_CBRT]) HAVE_CBRTF=1; AC_SUBST([HAVE_CBRTF]) HAVE_CBRTL=1; AC_SUBST([HAVE_CBRTL]) HAVE_COPYSIGN=1; AC_SUBST([HAVE_COPYSIGN]) HAVE_COPYSIGNL=1; AC_SUBST([HAVE_COPYSIGNL]) HAVE_COSF=1; AC_SUBST([HAVE_COSF]) HAVE_COSL=1; AC_SUBST([HAVE_COSL]) HAVE_COSHF=1; AC_SUBST([HAVE_COSHF]) HAVE_EXPF=1; AC_SUBST([HAVE_EXPF]) HAVE_EXPL=1; AC_SUBST([HAVE_EXPL]) HAVE_EXPM1=1; AC_SUBST([HAVE_EXPM1]) HAVE_EXPM1F=1; AC_SUBST([HAVE_EXPM1F]) HAVE_FABSF=1; AC_SUBST([HAVE_FABSF]) HAVE_FABSL=1; AC_SUBST([HAVE_FABSL]) HAVE_FMA=1; AC_SUBST([HAVE_FMA]) HAVE_FMAF=1; AC_SUBST([HAVE_FMAF]) HAVE_FMAL=1; AC_SUBST([HAVE_FMAL]) HAVE_FMODF=1; AC_SUBST([HAVE_FMODF]) HAVE_FMODL=1; AC_SUBST([HAVE_FMODL]) HAVE_FREXPF=1; AC_SUBST([HAVE_FREXPF]) HAVE_HYPOTF=1; AC_SUBST([HAVE_HYPOTF]) HAVE_HYPOTL=1; AC_SUBST([HAVE_HYPOTL]) HAVE_ILOGB=1; AC_SUBST([HAVE_ILOGB]) HAVE_ILOGBF=1; AC_SUBST([HAVE_ILOGBF]) HAVE_ILOGBL=1; AC_SUBST([HAVE_ILOGBL]) HAVE_ISNANF=1; AC_SUBST([HAVE_ISNANF]) HAVE_ISNAND=1; AC_SUBST([HAVE_ISNAND]) HAVE_ISNANL=1; AC_SUBST([HAVE_ISNANL]) HAVE_LDEXPF=1; AC_SUBST([HAVE_LDEXPF]) HAVE_LOGF=1; AC_SUBST([HAVE_LOGF]) HAVE_LOGL=1; AC_SUBST([HAVE_LOGL]) HAVE_LOG10F=1; AC_SUBST([HAVE_LOG10F]) HAVE_LOG10L=1; AC_SUBST([HAVE_LOG10L]) HAVE_LOG1P=1; AC_SUBST([HAVE_LOG1P]) HAVE_LOG1PF=1; AC_SUBST([HAVE_LOG1PF]) HAVE_LOG1PL=1; AC_SUBST([HAVE_LOG1PL]) HAVE_LOGBF=1; AC_SUBST([HAVE_LOGBF]) HAVE_LOGBL=1; AC_SUBST([HAVE_LOGBL]) HAVE_MODFF=1; AC_SUBST([HAVE_MODFF]) HAVE_MODFL=1; AC_SUBST([HAVE_MODFL]) HAVE_POWF=1; AC_SUBST([HAVE_POWF]) HAVE_REMAINDER=1; AC_SUBST([HAVE_REMAINDER]) HAVE_REMAINDERF=1; AC_SUBST([HAVE_REMAINDERF]) HAVE_RINT=1; AC_SUBST([HAVE_RINT]) HAVE_RINTL=1; AC_SUBST([HAVE_RINTL]) HAVE_SINF=1; AC_SUBST([HAVE_SINF]) HAVE_SINL=1; AC_SUBST([HAVE_SINL]) HAVE_SINHF=1; AC_SUBST([HAVE_SINHF]) HAVE_SQRTF=1; AC_SUBST([HAVE_SQRTF]) HAVE_SQRTL=1; AC_SUBST([HAVE_SQRTL]) HAVE_TANF=1; AC_SUBST([HAVE_TANF]) HAVE_TANL=1; AC_SUBST([HAVE_TANL]) HAVE_TANHF=1; AC_SUBST([HAVE_TANHF]) HAVE_DECL_ACOSL=1; AC_SUBST([HAVE_DECL_ACOSL]) HAVE_DECL_ASINL=1; AC_SUBST([HAVE_DECL_ASINL]) HAVE_DECL_ATANL=1; AC_SUBST([HAVE_DECL_ATANL]) HAVE_DECL_CBRTF=1; AC_SUBST([HAVE_DECL_CBRTF]) HAVE_DECL_CBRTL=1; AC_SUBST([HAVE_DECL_CBRTL]) HAVE_DECL_CEILF=1; AC_SUBST([HAVE_DECL_CEILF]) HAVE_DECL_CEILL=1; AC_SUBST([HAVE_DECL_CEILL]) HAVE_DECL_COPYSIGNF=1; AC_SUBST([HAVE_DECL_COPYSIGNF]) HAVE_DECL_COSL=1; AC_SUBST([HAVE_DECL_COSL]) HAVE_DECL_EXPL=1; AC_SUBST([HAVE_DECL_EXPL]) HAVE_DECL_EXP2=1; AC_SUBST([HAVE_DECL_EXP2]) HAVE_DECL_EXP2F=1; AC_SUBST([HAVE_DECL_EXP2F]) HAVE_DECL_EXP2L=1; AC_SUBST([HAVE_DECL_EXP2L]) HAVE_DECL_EXPM1L=1; AC_SUBST([HAVE_DECL_EXPM1L]) HAVE_DECL_FLOORF=1; AC_SUBST([HAVE_DECL_FLOORF]) HAVE_DECL_FLOORL=1; AC_SUBST([HAVE_DECL_FLOORL]) HAVE_DECL_FREXPL=1; AC_SUBST([HAVE_DECL_FREXPL]) HAVE_DECL_LDEXPL=1; AC_SUBST([HAVE_DECL_LDEXPL]) HAVE_DECL_LOGL=1; AC_SUBST([HAVE_DECL_LOGL]) HAVE_DECL_LOG10L=1; AC_SUBST([HAVE_DECL_LOG10L]) HAVE_DECL_LOG2=1; AC_SUBST([HAVE_DECL_LOG2]) HAVE_DECL_LOG2F=1; AC_SUBST([HAVE_DECL_LOG2F]) HAVE_DECL_LOG2L=1; AC_SUBST([HAVE_DECL_LOG2L]) HAVE_DECL_LOGB=1; AC_SUBST([HAVE_DECL_LOGB]) HAVE_DECL_REMAINDER=1; AC_SUBST([HAVE_DECL_REMAINDER]) HAVE_DECL_REMAINDERL=1; AC_SUBST([HAVE_DECL_REMAINDERL]) HAVE_DECL_RINTF=1; AC_SUBST([HAVE_DECL_RINTF]) HAVE_DECL_ROUND=1; AC_SUBST([HAVE_DECL_ROUND]) HAVE_DECL_ROUNDF=1; AC_SUBST([HAVE_DECL_ROUNDF]) HAVE_DECL_ROUNDL=1; AC_SUBST([HAVE_DECL_ROUNDL]) HAVE_DECL_SINL=1; AC_SUBST([HAVE_DECL_SINL]) HAVE_DECL_SQRTL=1; AC_SUBST([HAVE_DECL_SQRTL]) HAVE_DECL_TANL=1; AC_SUBST([HAVE_DECL_TANL]) HAVE_DECL_TRUNC=1; AC_SUBST([HAVE_DECL_TRUNC]) HAVE_DECL_TRUNCF=1; AC_SUBST([HAVE_DECL_TRUNCF]) HAVE_DECL_TRUNCL=1; AC_SUBST([HAVE_DECL_TRUNCL]) REPLACE_ACOSF=0; AC_SUBST([REPLACE_ACOSF]) REPLACE_ASINF=0; AC_SUBST([REPLACE_ASINF]) REPLACE_ATANF=0; AC_SUBST([REPLACE_ATANF]) REPLACE_ATAN2F=0; AC_SUBST([REPLACE_ATAN2F]) REPLACE_CBRTF=0; AC_SUBST([REPLACE_CBRTF]) REPLACE_CBRTL=0; AC_SUBST([REPLACE_CBRTL]) REPLACE_CEIL=0; AC_SUBST([REPLACE_CEIL]) REPLACE_CEILF=0; AC_SUBST([REPLACE_CEILF]) REPLACE_CEILL=0; AC_SUBST([REPLACE_CEILL]) REPLACE_COSF=0; AC_SUBST([REPLACE_COSF]) REPLACE_COSHF=0; AC_SUBST([REPLACE_COSHF]) REPLACE_EXPF=0; AC_SUBST([REPLACE_EXPF]) REPLACE_EXPM1=0; AC_SUBST([REPLACE_EXPM1]) REPLACE_EXPM1F=0; AC_SUBST([REPLACE_EXPM1F]) REPLACE_EXP2=0; AC_SUBST([REPLACE_EXP2]) REPLACE_EXP2L=0; AC_SUBST([REPLACE_EXP2L]) REPLACE_FABSL=0; AC_SUBST([REPLACE_FABSL]) REPLACE_FLOOR=0; AC_SUBST([REPLACE_FLOOR]) REPLACE_FLOORF=0; AC_SUBST([REPLACE_FLOORF]) REPLACE_FLOORL=0; AC_SUBST([REPLACE_FLOORL]) REPLACE_FMA=0; AC_SUBST([REPLACE_FMA]) REPLACE_FMAF=0; AC_SUBST([REPLACE_FMAF]) REPLACE_FMAL=0; AC_SUBST([REPLACE_FMAL]) REPLACE_FMOD=0; AC_SUBST([REPLACE_FMOD]) REPLACE_FMODF=0; AC_SUBST([REPLACE_FMODF]) REPLACE_FMODL=0; AC_SUBST([REPLACE_FMODL]) REPLACE_FREXPF=0; AC_SUBST([REPLACE_FREXPF]) REPLACE_FREXP=0; AC_SUBST([REPLACE_FREXP]) REPLACE_FREXPL=0; AC_SUBST([REPLACE_FREXPL]) REPLACE_HUGE_VAL=0; AC_SUBST([REPLACE_HUGE_VAL]) REPLACE_HYPOT=0; AC_SUBST([REPLACE_HYPOT]) REPLACE_HYPOTF=0; AC_SUBST([REPLACE_HYPOTF]) REPLACE_HYPOTL=0; AC_SUBST([REPLACE_HYPOTL]) REPLACE_ILOGB=0; AC_SUBST([REPLACE_ILOGB]) REPLACE_ILOGBF=0; AC_SUBST([REPLACE_ILOGBF]) REPLACE_ILOGBL=0; AC_SUBST([REPLACE_ILOGBL]) REPLACE_ISFINITE=0; AC_SUBST([REPLACE_ISFINITE]) REPLACE_ISINF=0; AC_SUBST([REPLACE_ISINF]) REPLACE_ISNAN=0; AC_SUBST([REPLACE_ISNAN]) REPLACE_LDEXPL=0; AC_SUBST([REPLACE_LDEXPL]) REPLACE_LOG=0; AC_SUBST([REPLACE_LOG]) REPLACE_LOGF=0; AC_SUBST([REPLACE_LOGF]) REPLACE_LOGL=0; AC_SUBST([REPLACE_LOGL]) REPLACE_LOG10=0; AC_SUBST([REPLACE_LOG10]) REPLACE_LOG10F=0; AC_SUBST([REPLACE_LOG10F]) REPLACE_LOG10L=0; AC_SUBST([REPLACE_LOG10L]) REPLACE_LOG1P=0; AC_SUBST([REPLACE_LOG1P]) REPLACE_LOG1PF=0; AC_SUBST([REPLACE_LOG1PF]) REPLACE_LOG1PL=0; AC_SUBST([REPLACE_LOG1PL]) REPLACE_LOG2=0; AC_SUBST([REPLACE_LOG2]) REPLACE_LOG2F=0; AC_SUBST([REPLACE_LOG2F]) REPLACE_LOG2L=0; AC_SUBST([REPLACE_LOG2L]) REPLACE_LOGB=0; AC_SUBST([REPLACE_LOGB]) REPLACE_LOGBF=0; AC_SUBST([REPLACE_LOGBF]) REPLACE_LOGBL=0; AC_SUBST([REPLACE_LOGBL]) REPLACE_MODF=0; AC_SUBST([REPLACE_MODF]) REPLACE_MODFF=0; AC_SUBST([REPLACE_MODFF]) REPLACE_MODFL=0; AC_SUBST([REPLACE_MODFL]) REPLACE_NAN=0; AC_SUBST([REPLACE_NAN]) REPLACE_REMAINDER=0; AC_SUBST([REPLACE_REMAINDER]) REPLACE_REMAINDERF=0; AC_SUBST([REPLACE_REMAINDERF]) REPLACE_REMAINDERL=0; AC_SUBST([REPLACE_REMAINDERL]) REPLACE_ROUND=0; AC_SUBST([REPLACE_ROUND]) REPLACE_ROUNDF=0; AC_SUBST([REPLACE_ROUNDF]) REPLACE_ROUNDL=0; AC_SUBST([REPLACE_ROUNDL]) REPLACE_SIGNBIT=0; AC_SUBST([REPLACE_SIGNBIT]) REPLACE_SIGNBIT_USING_GCC=0; AC_SUBST([REPLACE_SIGNBIT_USING_GCC]) REPLACE_SINF=0; AC_SUBST([REPLACE_SINF]) REPLACE_SINHF=0; AC_SUBST([REPLACE_SINHF]) REPLACE_SQRTF=0; AC_SUBST([REPLACE_SQRTF]) REPLACE_SQRTL=0; AC_SUBST([REPLACE_SQRTL]) REPLACE_TANF=0; AC_SUBST([REPLACE_TANF]) REPLACE_TANHF=0; AC_SUBST([REPLACE_TANHF]) REPLACE_TRUNC=0; AC_SUBST([REPLACE_TRUNC]) REPLACE_TRUNCF=0; AC_SUBST([REPLACE_TRUNCF]) REPLACE_TRUNCL=0; AC_SUBST([REPLACE_TRUNCL]) ]) # gl_LONG_DOUBLE_VS_DOUBLE # determines whether 'long double' and 'double' have the same representation. # Sets variable HAVE_SAME_LONG_DOUBLE_AS_DOUBLE to 0 or 1, and defines # HAVE_SAME_LONG_DOUBLE_AS_DOUBLE accordingly. # The currently known platforms where this is the case are: # Linux/HPPA, Minix 3.1.8, AIX 5, AIX 6 and 7 with xlc, MSVC 9. AC_DEFUN([gl_LONG_DOUBLE_VS_DOUBLE], [ AC_CACHE_CHECK([whether long double and double are the same], [gl_cv_long_double_equals_double], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include ]], [[typedef int check[sizeof (long double) == sizeof (double) && LDBL_MANT_DIG == DBL_MANT_DIG && LDBL_MAX_EXP == DBL_MAX_EXP && LDBL_MIN_EXP == DBL_MIN_EXP ? 1 : -1]; ]])], [gl_cv_long_double_equals_double=yes], [gl_cv_long_double_equals_double=no]) ]) if test $gl_cv_long_double_equals_double = yes; then AC_DEFINE([HAVE_SAME_LONG_DOUBLE_AS_DOUBLE], [1], [Define to 1 if 'long double' and 'double' have the same representation.]) HAVE_SAME_LONG_DOUBLE_AS_DOUBLE=1 else HAVE_SAME_LONG_DOUBLE_AS_DOUBLE=0 fi AC_SUBST([HAVE_SAME_LONG_DOUBLE_AS_DOUBLE]) ]) gnuastro-0.5/bootstrapped/m4/malloca.m40000644000175000017500000000110113217200022015017 00000000000000# malloca.m4 serial 1 dnl Copyright (C) 2003-2004, 2006-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_MALLOCA], [ dnl Use the autoconf tests for alloca(), but not the AC_SUBSTed variables dnl @ALLOCA@ and @LTALLOCA@. dnl gl_FUNC_ALLOCA dnl Already brought in by the module dependencies. AC_REQUIRE([gl_EEMALLOC]) AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) ]) gnuastro-0.5/bootstrapped/m4/malloc.m40000644000175000017500000000642413217200022014673 00000000000000# malloc.m4 serial 15 dnl Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. m4_version_prereq([2.70], [] ,[ # This is adapted with modifications from upstream Autoconf here: # https://git.savannah.gnu.org/cgit/autoconf.git/commit/?id=04be2b7a29d65d9a08e64e8e56e594c91749598c AC_DEFUN([_AC_FUNC_MALLOC_IF], [ AC_REQUIRE([AC_HEADER_STDC])dnl AC_REQUIRE([AC_CANONICAL_HOST])dnl for cross-compiles AC_CHECK_HEADERS([stdlib.h]) AC_CACHE_CHECK([for GNU libc compatible malloc], [ac_cv_func_malloc_0_nonnull], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#if defined STDC_HEADERS || defined HAVE_STDLIB_H # include #else char *malloc (); #endif ]], [[char *p = malloc (0); int result = !p; free (p); return result;]]) ], [ac_cv_func_malloc_0_nonnull=yes], [ac_cv_func_malloc_0_nonnull=no], [case "$host_os" in # Guess yes on platforms where we know the result. *-gnu* | freebsd* | netbsd* | openbsd* \ | hpux* | solaris* | cygwin* | mingw*) ac_cv_func_malloc_0_nonnull=yes ;; # If we don't know, assume the worst. *) ac_cv_func_malloc_0_nonnull=no ;; esac ]) ]) AS_IF([test $ac_cv_func_malloc_0_nonnull = yes], [$1], [$2]) ])# _AC_FUNC_MALLOC_IF ]) # gl_FUNC_MALLOC_GNU # ------------------ # Test whether 'malloc (0)' is handled like in GNU libc, and replace malloc if # it is not. AC_DEFUN([gl_FUNC_MALLOC_GNU], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) dnl _AC_FUNC_MALLOC_IF is defined in Autoconf. _AC_FUNC_MALLOC_IF( [AC_DEFINE([HAVE_MALLOC_GNU], [1], [Define to 1 if your system has a GNU libc compatible 'malloc' function, and to 0 otherwise.])], [AC_DEFINE([HAVE_MALLOC_GNU], [0]) REPLACE_MALLOC=1 ]) ]) # gl_FUNC_MALLOC_POSIX # -------------------- # Test whether 'malloc' is POSIX compliant (sets errno to ENOMEM when it # fails), and replace malloc if it is not. AC_DEFUN([gl_FUNC_MALLOC_POSIX], [ AC_REQUIRE([gl_STDLIB_H_DEFAULTS]) AC_REQUIRE([gl_CHECK_MALLOC_POSIX]) if test $gl_cv_func_malloc_posix = yes; then AC_DEFINE([HAVE_MALLOC_POSIX], [1], [Define if the 'malloc' function is POSIX compliant.]) else REPLACE_MALLOC=1 fi ]) # Test whether malloc, realloc, calloc are POSIX compliant, # Set gl_cv_func_malloc_posix to yes or no accordingly. AC_DEFUN([gl_CHECK_MALLOC_POSIX], [ AC_CACHE_CHECK([whether malloc, realloc, calloc are POSIX compliant], [gl_cv_func_malloc_posix], [ dnl It is too dangerous to try to allocate a large amount of memory: dnl some systems go to their knees when you do that. So assume that dnl all Unix implementations of the function are POSIX compliant. AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[]], [[#if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ choke me #endif ]])], [gl_cv_func_malloc_posix=yes], [gl_cv_func_malloc_posix=no]) ]) ]) gnuastro-0.5/bootstrapped/m4/lt~obsolete.m40000644000175000017500000001377413217177774016037 00000000000000# lt~obsolete.m4 -- aclocal satisfying obsolete definitions. -*-Autoconf-*- # # Copyright (C) 2004-2005, 2007, 2009, 2011-2017 Free Software # Foundation, Inc. # Written by Scott James Remnant, 2004. # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # serial 5 lt~obsolete.m4 # These exist entirely to fool aclocal when bootstrapping libtool. # # In the past libtool.m4 has provided macros via AC_DEFUN (or AU_DEFUN), # which have later been changed to m4_define as they aren't part of the # exported API, or moved to Autoconf or Automake where they belong. # # The trouble is, aclocal is a bit thick. It'll see the old AC_DEFUN # in /usr/share/aclocal/libtool.m4 and remember it, then when it sees us # using a macro with the same name in our local m4/libtool.m4 it'll # pull the old libtool.m4 in (it doesn't see our shiny new m4_define # and doesn't know about Autoconf macros at all.) # # So we provide this file, which has a silly filename so it's always # included after everything else. This provides aclocal with the # AC_DEFUNs it wants, but when m4 processes it, it doesn't do anything # because those macros already exist, or will be overwritten later. # We use AC_DEFUN over AU_DEFUN for compatibility with aclocal-1.6. # # Anytime we withdraw an AC_DEFUN or AU_DEFUN, remember to add it here. # Yes, that means every name once taken will need to remain here until # we give up compatibility with versions before 1.7, at which point # we need to keep only those names which we still refer to. # This is to help aclocal find these macros, as it can't see m4_define. AC_DEFUN([LTOBSOLETE_VERSION], [m4_if([1])]) m4_ifndef([AC_LIBTOOL_LINKER_OPTION], [AC_DEFUN([AC_LIBTOOL_LINKER_OPTION])]) m4_ifndef([AC_PROG_EGREP], [AC_DEFUN([AC_PROG_EGREP])]) m4_ifndef([_LT_AC_PROG_ECHO_BACKSLASH], [AC_DEFUN([_LT_AC_PROG_ECHO_BACKSLASH])]) m4_ifndef([_LT_AC_SHELL_INIT], [AC_DEFUN([_LT_AC_SHELL_INIT])]) m4_ifndef([_LT_AC_SYS_LIBPATH_AIX], [AC_DEFUN([_LT_AC_SYS_LIBPATH_AIX])]) m4_ifndef([_LT_PROG_LTMAIN], [AC_DEFUN([_LT_PROG_LTMAIN])]) m4_ifndef([_LT_AC_TAGVAR], [AC_DEFUN([_LT_AC_TAGVAR])]) m4_ifndef([AC_LTDL_ENABLE_INSTALL], [AC_DEFUN([AC_LTDL_ENABLE_INSTALL])]) m4_ifndef([AC_LTDL_PREOPEN], [AC_DEFUN([AC_LTDL_PREOPEN])]) m4_ifndef([_LT_AC_SYS_COMPILER], [AC_DEFUN([_LT_AC_SYS_COMPILER])]) m4_ifndef([_LT_AC_LOCK], [AC_DEFUN([_LT_AC_LOCK])]) m4_ifndef([AC_LIBTOOL_SYS_OLD_ARCHIVE], [AC_DEFUN([AC_LIBTOOL_SYS_OLD_ARCHIVE])]) m4_ifndef([_LT_AC_TRY_DLOPEN_SELF], [AC_DEFUN([_LT_AC_TRY_DLOPEN_SELF])]) m4_ifndef([AC_LIBTOOL_PROG_CC_C_O], [AC_DEFUN([AC_LIBTOOL_PROG_CC_C_O])]) m4_ifndef([AC_LIBTOOL_SYS_HARD_LINK_LOCKS], [AC_DEFUN([AC_LIBTOOL_SYS_HARD_LINK_LOCKS])]) m4_ifndef([AC_LIBTOOL_OBJDIR], [AC_DEFUN([AC_LIBTOOL_OBJDIR])]) m4_ifndef([AC_LTDL_OBJDIR], [AC_DEFUN([AC_LTDL_OBJDIR])]) m4_ifndef([AC_LIBTOOL_PROG_LD_HARDCODE_LIBPATH], [AC_DEFUN([AC_LIBTOOL_PROG_LD_HARDCODE_LIBPATH])]) m4_ifndef([AC_LIBTOOL_SYS_LIB_STRIP], [AC_DEFUN([AC_LIBTOOL_SYS_LIB_STRIP])]) m4_ifndef([AC_PATH_MAGIC], [AC_DEFUN([AC_PATH_MAGIC])]) m4_ifndef([AC_PROG_LD_GNU], [AC_DEFUN([AC_PROG_LD_GNU])]) m4_ifndef([AC_PROG_LD_RELOAD_FLAG], [AC_DEFUN([AC_PROG_LD_RELOAD_FLAG])]) m4_ifndef([AC_DEPLIBS_CHECK_METHOD], [AC_DEFUN([AC_DEPLIBS_CHECK_METHOD])]) m4_ifndef([AC_LIBTOOL_PROG_COMPILER_NO_RTTI], [AC_DEFUN([AC_LIBTOOL_PROG_COMPILER_NO_RTTI])]) m4_ifndef([AC_LIBTOOL_SYS_GLOBAL_SYMBOL_PIPE], [AC_DEFUN([AC_LIBTOOL_SYS_GLOBAL_SYMBOL_PIPE])]) m4_ifndef([AC_LIBTOOL_PROG_COMPILER_PIC], [AC_DEFUN([AC_LIBTOOL_PROG_COMPILER_PIC])]) m4_ifndef([AC_LIBTOOL_PROG_LD_SHLIBS], [AC_DEFUN([AC_LIBTOOL_PROG_LD_SHLIBS])]) m4_ifndef([AC_LIBTOOL_POSTDEP_PREDEP], [AC_DEFUN([AC_LIBTOOL_POSTDEP_PREDEP])]) m4_ifndef([LT_AC_PROG_EGREP], [AC_DEFUN([LT_AC_PROG_EGREP])]) m4_ifndef([LT_AC_PROG_SED], [AC_DEFUN([LT_AC_PROG_SED])]) m4_ifndef([_LT_CC_BASENAME], [AC_DEFUN([_LT_CC_BASENAME])]) m4_ifndef([_LT_COMPILER_BOILERPLATE], [AC_DEFUN([_LT_COMPILER_BOILERPLATE])]) m4_ifndef([_LT_LINKER_BOILERPLATE], [AC_DEFUN([_LT_LINKER_BOILERPLATE])]) m4_ifndef([_AC_PROG_LIBTOOL], [AC_DEFUN([_AC_PROG_LIBTOOL])]) m4_ifndef([AC_LIBTOOL_SETUP], [AC_DEFUN([AC_LIBTOOL_SETUP])]) m4_ifndef([_LT_AC_CHECK_DLFCN], [AC_DEFUN([_LT_AC_CHECK_DLFCN])]) m4_ifndef([AC_LIBTOOL_SYS_DYNAMIC_LINKER], [AC_DEFUN([AC_LIBTOOL_SYS_DYNAMIC_LINKER])]) m4_ifndef([_LT_AC_TAGCONFIG], [AC_DEFUN([_LT_AC_TAGCONFIG])]) m4_ifndef([AC_DISABLE_FAST_INSTALL], [AC_DEFUN([AC_DISABLE_FAST_INSTALL])]) m4_ifndef([_LT_AC_LANG_CXX], [AC_DEFUN([_LT_AC_LANG_CXX])]) m4_ifndef([_LT_AC_LANG_F77], [AC_DEFUN([_LT_AC_LANG_F77])]) m4_ifndef([_LT_AC_LANG_GCJ], [AC_DEFUN([_LT_AC_LANG_GCJ])]) m4_ifndef([AC_LIBTOOL_LANG_C_CONFIG], [AC_DEFUN([AC_LIBTOOL_LANG_C_CONFIG])]) m4_ifndef([_LT_AC_LANG_C_CONFIG], [AC_DEFUN([_LT_AC_LANG_C_CONFIG])]) m4_ifndef([AC_LIBTOOL_LANG_CXX_CONFIG], [AC_DEFUN([AC_LIBTOOL_LANG_CXX_CONFIG])]) m4_ifndef([_LT_AC_LANG_CXX_CONFIG], [AC_DEFUN([_LT_AC_LANG_CXX_CONFIG])]) m4_ifndef([AC_LIBTOOL_LANG_F77_CONFIG], [AC_DEFUN([AC_LIBTOOL_LANG_F77_CONFIG])]) m4_ifndef([_LT_AC_LANG_F77_CONFIG], [AC_DEFUN([_LT_AC_LANG_F77_CONFIG])]) m4_ifndef([AC_LIBTOOL_LANG_GCJ_CONFIG], [AC_DEFUN([AC_LIBTOOL_LANG_GCJ_CONFIG])]) m4_ifndef([_LT_AC_LANG_GCJ_CONFIG], [AC_DEFUN([_LT_AC_LANG_GCJ_CONFIG])]) m4_ifndef([AC_LIBTOOL_LANG_RC_CONFIG], [AC_DEFUN([AC_LIBTOOL_LANG_RC_CONFIG])]) m4_ifndef([_LT_AC_LANG_RC_CONFIG], [AC_DEFUN([_LT_AC_LANG_RC_CONFIG])]) m4_ifndef([AC_LIBTOOL_CONFIG], [AC_DEFUN([AC_LIBTOOL_CONFIG])]) m4_ifndef([_LT_AC_FILE_LTDLL_C], [AC_DEFUN([_LT_AC_FILE_LTDLL_C])]) m4_ifndef([_LT_REQUIRED_DARWIN_CHECKS], [AC_DEFUN([_LT_REQUIRED_DARWIN_CHECKS])]) m4_ifndef([_LT_AC_PROG_CXXCPP], [AC_DEFUN([_LT_AC_PROG_CXXCPP])]) m4_ifndef([_LT_PREPARE_SED_QUOTE_VARS], [AC_DEFUN([_LT_PREPARE_SED_QUOTE_VARS])]) m4_ifndef([_LT_PROG_ECHO_BACKSLASH], [AC_DEFUN([_LT_PROG_ECHO_BACKSLASH])]) m4_ifndef([_LT_PROG_F77], [AC_DEFUN([_LT_PROG_F77])]) m4_ifndef([_LT_PROG_FC], [AC_DEFUN([_LT_PROG_FC])]) m4_ifndef([_LT_PROG_CXX], [AC_DEFUN([_LT_PROG_CXX])]) gnuastro-0.5/bootstrapped/m4/ltversion.m40000644000175000017500000000133513217177774015500 00000000000000# ltversion.m4 -- version numbers -*- Autoconf -*- # # Copyright (C) 2004, 2011-2017 Free Software Foundation, Inc. # Written by Scott James Remnant, 2004 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # @configure_input@ # serial 4219 ltversion.m4 # This file is part of GNU Libtool m4_define([LT_PACKAGE_VERSION], [2.4.6.40-6ca5-dirty]) m4_define([LT_PACKAGE_REVISION], [2.4.6.40]) AC_DEFUN([LTVERSION_VERSION], [macro_version='2.4.6.40-6ca5-dirty' macro_revision='2.4.6.40' _LT_DECL(, macro_version, 0, [Which release of libtool.m4 was used?]) _LT_DECL(, macro_revision, 0) ]) gnuastro-0.5/bootstrapped/m4/ltsugar.m40000644000175000017500000001044013217177774015131 00000000000000# ltsugar.m4 -- libtool m4 base layer. -*-Autoconf-*- # # Copyright (C) 2004-2005, 2007-2008, 2011-2017 Free Software # Foundation, Inc. # Written by Gary V. Vaughan, 2004 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # serial 6 ltsugar.m4 # This is to help aclocal find these macros, as it can't see m4_define. AC_DEFUN([LTSUGAR_VERSION], [m4_if([0.1])]) # lt_join(SEP, ARG1, [ARG2...]) # ----------------------------- # Produce ARG1SEPARG2...SEPARGn, omitting [] arguments and their # associated separator. # Needed until we can rely on m4_join from Autoconf 2.62, since all earlier # versions in m4sugar had bugs. m4_define([lt_join], [m4_if([$#], [1], [], [$#], [2], [[$2]], [m4_if([$2], [], [], [[$2]_])$0([$1], m4_shift(m4_shift($@)))])]) m4_define([_lt_join], [m4_if([$#$2], [2], [], [m4_if([$2], [], [], [[$1$2]])$0([$1], m4_shift(m4_shift($@)))])]) # lt_car(LIST) # lt_cdr(LIST) # ------------ # Manipulate m4 lists. # These macros are necessary as long as will still need to support # Autoconf-2.59, which quotes differently. m4_define([lt_car], [[$1]]) m4_define([lt_cdr], [m4_if([$#], 0, [m4_fatal([$0: cannot be called without arguments])], [$#], 1, [], [m4_dquote(m4_shift($@))])]) m4_define([lt_unquote], $1) # lt_append(MACRO-NAME, STRING, [SEPARATOR]) # ------------------------------------------ # Redefine MACRO-NAME to hold its former content plus 'SEPARATOR''STRING'. # Note that neither SEPARATOR nor STRING are expanded; they are appended # to MACRO-NAME as is (leaving the expansion for when MACRO-NAME is invoked). # No SEPARATOR is output if MACRO-NAME was previously undefined (different # than defined and empty). # # This macro is needed until we can rely on Autoconf 2.62, since earlier # versions of m4sugar mistakenly expanded SEPARATOR but not STRING. m4_define([lt_append], [m4_define([$1], m4_ifdef([$1], [m4_defn([$1])[$3]])[$2])]) # lt_combine(SEP, PREFIX-LIST, INFIX, SUFFIX1, [SUFFIX2...]) # ---------------------------------------------------------- # Produce a SEP delimited list of all paired combinations of elements of # PREFIX-LIST with SUFFIX1 through SUFFIXn. Each element of the list # has the form PREFIXmINFIXSUFFIXn. # Needed until we can rely on m4_combine added in Autoconf 2.62. m4_define([lt_combine], [m4_if(m4_eval([$# > 3]), [1], [m4_pushdef([_Lt_sep], [m4_define([_Lt_sep], m4_defn([lt_car]))])]]dnl [[m4_foreach([_Lt_prefix], [$2], [m4_foreach([_Lt_suffix], ]m4_dquote(m4_dquote(m4_shift(m4_shift(m4_shift($@)))))[, [_Lt_sep([$1])[]m4_defn([_Lt_prefix])[$3]m4_defn([_Lt_suffix])])])])]) # lt_if_append_uniq(MACRO-NAME, VARNAME, [SEPARATOR], [UNIQ], [NOT-UNIQ]) # ----------------------------------------------------------------------- # Iff MACRO-NAME does not yet contain VARNAME, then append it (delimited # by SEPARATOR if supplied) and expand UNIQ, else NOT-UNIQ. m4_define([lt_if_append_uniq], [m4_ifdef([$1], [m4_if(m4_index([$3]m4_defn([$1])[$3], [$3$2$3]), [-1], [lt_append([$1], [$2], [$3])$4], [$5])], [lt_append([$1], [$2], [$3])$4])]) # lt_dict_add(DICT, KEY, VALUE) # ----------------------------- m4_define([lt_dict_add], [m4_define([$1($2)], [$3])]) # lt_dict_add_subkey(DICT, KEY, SUBKEY, VALUE) # -------------------------------------------- m4_define([lt_dict_add_subkey], [m4_define([$1($2:$3)], [$4])]) # lt_dict_fetch(DICT, KEY, [SUBKEY]) # ---------------------------------- m4_define([lt_dict_fetch], [m4_ifval([$3], m4_ifdef([$1($2:$3)], [m4_defn([$1($2:$3)])]), m4_ifdef([$1($2)], [m4_defn([$1($2)])]))]) # lt_if_dict_fetch(DICT, KEY, [SUBKEY], VALUE, IF-TRUE, [IF-FALSE]) # ----------------------------------------------------------------- m4_define([lt_if_dict_fetch], [m4_if(lt_dict_fetch([$1], [$2], [$3]), [$4], [$5], [$6])]) # lt_dict_filter(DICT, [SUBKEY], VALUE, [SEPARATOR], KEY, [...]) # -------------------------------------------------------------- m4_define([lt_dict_filter], [m4_if([$5], [], [], [lt_join(m4_quote(m4_default([$4], [[, ]])), lt_unquote(m4_split(m4_normalize(m4_foreach(_Lt_key, lt_car([m4_shiftn(4, $@)]), [lt_if_dict_fetch([$1], _Lt_key, [$2], [$3], [_Lt_key ])])))))])[]dnl ]) gnuastro-0.5/bootstrapped/m4/ltoptions.m40000644000175000017500000003426213217177774015513 00000000000000# Helper functions for option handling. -*- Autoconf -*- # # Copyright (C) 2004-2005, 2007-2009, 2011-2017 Free Software # Foundation, Inc. # Written by Gary V. Vaughan, 2004 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. # serial 8 ltoptions.m4 # This is to help aclocal find these macros, as it can't see m4_define. AC_DEFUN([LTOPTIONS_VERSION], [m4_if([1])]) # _LT_MANGLE_OPTION(MACRO-NAME, OPTION-NAME) # ------------------------------------------ m4_define([_LT_MANGLE_OPTION], [[_LT_OPTION_]m4_bpatsubst($1__$2, [[^a-zA-Z0-9_]], [_])]) # _LT_SET_OPTION(MACRO-NAME, OPTION-NAME) # --------------------------------------- # Set option OPTION-NAME for macro MACRO-NAME, and if there is a # matching handler defined, dispatch to it. Other OPTION-NAMEs are # saved as a flag. m4_define([_LT_SET_OPTION], [m4_define(_LT_MANGLE_OPTION([$1], [$2]))dnl m4_ifdef(_LT_MANGLE_DEFUN([$1], [$2]), _LT_MANGLE_DEFUN([$1], [$2]), [m4_warning([Unknown $1 option '$2'])])[]dnl ]) # _LT_IF_OPTION(MACRO-NAME, OPTION-NAME, IF-SET, [IF-NOT-SET]) # ------------------------------------------------------------ # Execute IF-SET if OPTION is set, IF-NOT-SET otherwise. m4_define([_LT_IF_OPTION], [m4_ifdef(_LT_MANGLE_OPTION([$1], [$2]), [$3], [$4])]) # _LT_UNLESS_OPTIONS(MACRO-NAME, OPTION-LIST, IF-NOT-SET) # ------------------------------------------------------- # Execute IF-NOT-SET unless all options in OPTION-LIST for MACRO-NAME # are set. m4_define([_LT_UNLESS_OPTIONS], [m4_foreach([_LT_Option], m4_split(m4_normalize([$2])), [m4_ifdef(_LT_MANGLE_OPTION([$1], _LT_Option), [m4_define([$0_found])])])[]dnl m4_ifdef([$0_found], [m4_undefine([$0_found])], [$3 ])[]dnl ]) # _LT_SET_OPTIONS(MACRO-NAME, OPTION-LIST) # ---------------------------------------- # OPTION-LIST is a space-separated list of Libtool options associated # with MACRO-NAME. If any OPTION has a matching handler declared with # LT_OPTION_DEFINE, dispatch to that macro; otherwise complain about # the unknown option and exit. m4_defun([_LT_SET_OPTIONS], [# Set options m4_foreach([_LT_Option], m4_split(m4_normalize([$2])), [_LT_SET_OPTION([$1], _LT_Option)]) m4_if([$1],[LT_INIT],[ dnl dnl Simply set some default values (i.e off) if boolean options were not dnl specified: _LT_UNLESS_OPTIONS([LT_INIT], [dlopen], [enable_dlopen=no ]) _LT_UNLESS_OPTIONS([LT_INIT], [win32-dll], [enable_win32_dll=no ]) dnl dnl If no reference was made to various pairs of opposing options, then dnl we run the default mode handler for the pair. For example, if neither dnl 'shared' nor 'disable-shared' was passed, we enable building of shared dnl archives by default: _LT_UNLESS_OPTIONS([LT_INIT], [shared disable-shared], [_LT_ENABLE_SHARED]) _LT_UNLESS_OPTIONS([LT_INIT], [static disable-static], [_LT_ENABLE_STATIC]) _LT_UNLESS_OPTIONS([LT_INIT], [pic-only no-pic], [_LT_WITH_PIC]) _LT_UNLESS_OPTIONS([LT_INIT], [fast-install disable-fast-install], [_LT_ENABLE_FAST_INSTALL]) _LT_UNLESS_OPTIONS([LT_INIT], [aix-soname=aix aix-soname=both aix-soname=svr4], [_LT_WITH_AIX_SONAME([aix])]) ]) ])# _LT_SET_OPTIONS ## --------------------------------- ## ## Macros to handle LT_INIT options. ## ## --------------------------------- ## # _LT_MANGLE_DEFUN(MACRO-NAME, OPTION-NAME) # ----------------------------------------- m4_define([_LT_MANGLE_DEFUN], [[_LT_OPTION_DEFUN_]m4_bpatsubst(m4_toupper([$1__$2]), [[^A-Z0-9_]], [_])]) # LT_OPTION_DEFINE(MACRO-NAME, OPTION-NAME, CODE) # ----------------------------------------------- m4_define([LT_OPTION_DEFINE], [m4_define(_LT_MANGLE_DEFUN([$1], [$2]), [$3])[]dnl ])# LT_OPTION_DEFINE # dlopen # ------ LT_OPTION_DEFINE([LT_INIT], [dlopen], [enable_dlopen=yes ]) AU_DEFUN([AC_LIBTOOL_DLOPEN], [_LT_SET_OPTION([LT_INIT], [dlopen]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'dlopen' option into LT_INIT's first parameter.]) ]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_DLOPEN], []) # win32-dll # --------- # Declare package support for building win32 dll's. LT_OPTION_DEFINE([LT_INIT], [win32-dll], [enable_win32_dll=yes case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-cegcc*) AC_CHECK_TOOL(AS, as, false) AC_CHECK_TOOL(DLLTOOL, dlltool, false) AC_CHECK_TOOL(OBJDUMP, objdump, false) ;; esac test -z "$AS" && AS=as _LT_DECL([], [AS], [1], [Assembler program])dnl test -z "$DLLTOOL" && DLLTOOL=dlltool _LT_DECL([], [DLLTOOL], [1], [DLL creation program])dnl test -z "$OBJDUMP" && OBJDUMP=objdump _LT_DECL([], [OBJDUMP], [1], [Object dumper program])dnl ])# win32-dll AU_DEFUN([AC_LIBTOOL_WIN32_DLL], [AC_REQUIRE([AC_CANONICAL_HOST])dnl _LT_SET_OPTION([LT_INIT], [win32-dll]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'win32-dll' option into LT_INIT's first parameter.]) ]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_WIN32_DLL], []) # _LT_ENABLE_SHARED([DEFAULT]) # ---------------------------- # implement the --enable-shared flag, and supports the 'shared' and # 'disable-shared' LT_INIT options. # DEFAULT is either 'yes' or 'no'. If omitted, it defaults to 'yes'. m4_define([_LT_ENABLE_SHARED], [m4_define([_LT_ENABLE_SHARED_DEFAULT], [m4_if($1, no, no, yes)])dnl AC_ARG_ENABLE([shared], [AS_HELP_STRING([--enable-shared@<:@=PKGS@:>@], [build shared libraries @<:@default=]_LT_ENABLE_SHARED_DEFAULT[@:>@])], [p=${PACKAGE-default} case $enableval in yes) enable_shared=yes ;; no) enable_shared=no ;; *) enable_shared=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_shared=yes fi done IFS=$lt_save_ifs ;; esac], [enable_shared=]_LT_ENABLE_SHARED_DEFAULT) _LT_DECL([build_libtool_libs], [enable_shared], [0], [Whether or not to build shared libraries]) ])# _LT_ENABLE_SHARED LT_OPTION_DEFINE([LT_INIT], [shared], [_LT_ENABLE_SHARED([yes])]) LT_OPTION_DEFINE([LT_INIT], [disable-shared], [_LT_ENABLE_SHARED([no])]) # Old names: AC_DEFUN([AC_ENABLE_SHARED], [_LT_SET_OPTION([LT_INIT], m4_if([$1], [no], [disable-])[shared]) ]) AC_DEFUN([AC_DISABLE_SHARED], [_LT_SET_OPTION([LT_INIT], [disable-shared]) ]) AU_DEFUN([AM_ENABLE_SHARED], [AC_ENABLE_SHARED($@)]) AU_DEFUN([AM_DISABLE_SHARED], [AC_DISABLE_SHARED($@)]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AM_ENABLE_SHARED], []) dnl AC_DEFUN([AM_DISABLE_SHARED], []) # _LT_ENABLE_STATIC([DEFAULT]) # ---------------------------- # implement the --enable-static flag, and support the 'static' and # 'disable-static' LT_INIT options. # DEFAULT is either 'yes' or 'no'. If omitted, it defaults to 'yes'. m4_define([_LT_ENABLE_STATIC], [m4_define([_LT_ENABLE_STATIC_DEFAULT], [m4_if($1, no, no, yes)])dnl AC_ARG_ENABLE([static], [AS_HELP_STRING([--enable-static@<:@=PKGS@:>@], [build static libraries @<:@default=]_LT_ENABLE_STATIC_DEFAULT[@:>@])], [p=${PACKAGE-default} case $enableval in yes) enable_static=yes ;; no) enable_static=no ;; *) enable_static=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_static=yes fi done IFS=$lt_save_ifs ;; esac], [enable_static=]_LT_ENABLE_STATIC_DEFAULT) _LT_DECL([build_old_libs], [enable_static], [0], [Whether or not to build static libraries]) ])# _LT_ENABLE_STATIC LT_OPTION_DEFINE([LT_INIT], [static], [_LT_ENABLE_STATIC([yes])]) LT_OPTION_DEFINE([LT_INIT], [disable-static], [_LT_ENABLE_STATIC([no])]) # Old names: AC_DEFUN([AC_ENABLE_STATIC], [_LT_SET_OPTION([LT_INIT], m4_if([$1], [no], [disable-])[static]) ]) AC_DEFUN([AC_DISABLE_STATIC], [_LT_SET_OPTION([LT_INIT], [disable-static]) ]) AU_DEFUN([AM_ENABLE_STATIC], [AC_ENABLE_STATIC($@)]) AU_DEFUN([AM_DISABLE_STATIC], [AC_DISABLE_STATIC($@)]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AM_ENABLE_STATIC], []) dnl AC_DEFUN([AM_DISABLE_STATIC], []) # _LT_ENABLE_FAST_INSTALL([DEFAULT]) # ---------------------------------- # implement the --enable-fast-install flag, and support the 'fast-install' # and 'disable-fast-install' LT_INIT options. # DEFAULT is either 'yes' or 'no'. If omitted, it defaults to 'yes'. m4_define([_LT_ENABLE_FAST_INSTALL], [m4_define([_LT_ENABLE_FAST_INSTALL_DEFAULT], [m4_if($1, no, no, yes)])dnl AC_ARG_ENABLE([fast-install], [AS_HELP_STRING([--enable-fast-install@<:@=PKGS@:>@], [optimize for fast installation @<:@default=]_LT_ENABLE_FAST_INSTALL_DEFAULT[@:>@])], [p=${PACKAGE-default} case $enableval in yes) enable_fast_install=yes ;; no) enable_fast_install=no ;; *) enable_fast_install=no # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for pkg in $enableval; do IFS=$lt_save_ifs if test "X$pkg" = "X$p"; then enable_fast_install=yes fi done IFS=$lt_save_ifs ;; esac], [enable_fast_install=]_LT_ENABLE_FAST_INSTALL_DEFAULT) _LT_DECL([fast_install], [enable_fast_install], [0], [Whether or not to optimize for fast installation])dnl ])# _LT_ENABLE_FAST_INSTALL LT_OPTION_DEFINE([LT_INIT], [fast-install], [_LT_ENABLE_FAST_INSTALL([yes])]) LT_OPTION_DEFINE([LT_INIT], [disable-fast-install], [_LT_ENABLE_FAST_INSTALL([no])]) # Old names: AU_DEFUN([AC_ENABLE_FAST_INSTALL], [_LT_SET_OPTION([LT_INIT], m4_if([$1], [no], [disable-])[fast-install]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'fast-install' option into LT_INIT's first parameter.]) ]) AU_DEFUN([AC_DISABLE_FAST_INSTALL], [_LT_SET_OPTION([LT_INIT], [disable-fast-install]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'disable-fast-install' option into LT_INIT's first parameter.]) ]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_ENABLE_FAST_INSTALL], []) dnl AC_DEFUN([AM_DISABLE_FAST_INSTALL], []) # _LT_WITH_AIX_SONAME([DEFAULT]) # ---------------------------------- # implement the --with-aix-soname flag, and support the `aix-soname=aix' # and `aix-soname=both' and `aix-soname=svr4' LT_INIT options. DEFAULT # is either `aix', `both' or `svr4'. If omitted, it defaults to `aix'. m4_define([_LT_WITH_AIX_SONAME], [m4_define([_LT_WITH_AIX_SONAME_DEFAULT], [m4_if($1, svr4, svr4, m4_if($1, both, both, aix))])dnl shared_archive_member_spec= case $host,$enable_shared in power*-*-aix[[5-9]]*,yes) AC_MSG_CHECKING([which variant of shared library versioning to provide]) AC_ARG_WITH([aix-soname], [AS_HELP_STRING([--with-aix-soname=aix|svr4|both], [shared library versioning (aka "SONAME") variant to provide on AIX, @<:@default=]_LT_WITH_AIX_SONAME_DEFAULT[@:>@.])], [case $withval in aix|svr4|both) ;; *) AC_MSG_ERROR([Unknown argument to --with-aix-soname]) ;; esac lt_cv_with_aix_soname=$with_aix_soname], [AC_CACHE_VAL([lt_cv_with_aix_soname], [lt_cv_with_aix_soname=]_LT_WITH_AIX_SONAME_DEFAULT) with_aix_soname=$lt_cv_with_aix_soname]) AC_MSG_RESULT([$with_aix_soname]) if test aix != "$with_aix_soname"; then # For the AIX way of multilib, we name the shared archive member # based on the bitwidth used, traditionally 'shr.o' or 'shr_64.o', # and 'shr.imp' or 'shr_64.imp', respectively, for the Import File. # Even when GNU compilers ignore OBJECT_MODE but need '-maix64' flag, # the AIX toolchain works better with OBJECT_MODE set (default 32). if test 64 = "${OBJECT_MODE-32}"; then shared_archive_member_spec=shr_64 else shared_archive_member_spec=shr fi fi ;; *) with_aix_soname=aix ;; esac _LT_DECL([], [shared_archive_member_spec], [0], [Shared archive member basename, for filename based shared library versioning on AIX])dnl ])# _LT_WITH_AIX_SONAME LT_OPTION_DEFINE([LT_INIT], [aix-soname=aix], [_LT_WITH_AIX_SONAME([aix])]) LT_OPTION_DEFINE([LT_INIT], [aix-soname=both], [_LT_WITH_AIX_SONAME([both])]) LT_OPTION_DEFINE([LT_INIT], [aix-soname=svr4], [_LT_WITH_AIX_SONAME([svr4])]) # _LT_WITH_PIC([MODE]) # -------------------- # implement the --with-pic flag, and support the 'pic-only' and 'no-pic' # LT_INIT options. # MODE is either 'yes' or 'no'. If omitted, it defaults to 'both'. m4_define([_LT_WITH_PIC], [AC_ARG_WITH([pic], [AS_HELP_STRING([--with-pic@<:@=PKGS@:>@], [try to use only PIC/non-PIC objects @<:@default=use both@:>@])], [lt_p=${PACKAGE-default} case $withval in yes|no) pic_mode=$withval ;; *) pic_mode=default # Look at the argument we got. We use all the common list separators. lt_save_ifs=$IFS; IFS=$IFS$PATH_SEPARATOR, for lt_pkg in $withval; do IFS=$lt_save_ifs if test "X$lt_pkg" = "X$lt_p"; then pic_mode=yes fi done IFS=$lt_save_ifs ;; esac], [pic_mode=m4_default([$1], [default])]) _LT_DECL([], [pic_mode], [0], [What type of objects to build])dnl ])# _LT_WITH_PIC LT_OPTION_DEFINE([LT_INIT], [pic-only], [_LT_WITH_PIC([yes])]) LT_OPTION_DEFINE([LT_INIT], [no-pic], [_LT_WITH_PIC([no])]) # Old name: AU_DEFUN([AC_LIBTOOL_PICMODE], [_LT_SET_OPTION([LT_INIT], [pic-only]) AC_DIAGNOSE([obsolete], [$0: Remove this warning and the call to _LT_SET_OPTION when you put the 'pic-only' option into LT_INIT's first parameter.]) ]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_PICMODE], []) ## ----------------- ## ## LTDL_INIT Options ## ## ----------------- ## m4_define([_LTDL_MODE], []) LT_OPTION_DEFINE([LTDL_INIT], [nonrecursive], [m4_define([_LTDL_MODE], [nonrecursive])]) LT_OPTION_DEFINE([LTDL_INIT], [recursive], [m4_define([_LTDL_MODE], [recursive])]) LT_OPTION_DEFINE([LTDL_INIT], [subproject], [m4_define([_LTDL_MODE], [subproject])]) m4_define([_LTDL_TYPE], []) LT_OPTION_DEFINE([LTDL_INIT], [installable], [m4_define([_LTDL_TYPE], [installable])]) LT_OPTION_DEFINE([LTDL_INIT], [convenience], [m4_define([_LTDL_TYPE], [convenience])]) gnuastro-0.5/bootstrapped/m4/lstat.m40000644000175000017500000000516313217200022014552 00000000000000# serial 30 # Copyright (C) 1997-2001, 2003-2017 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl From Jim Meyering. AC_DEFUN([gl_FUNC_LSTAT], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) dnl If lstat does not exist, the replacement does dnl "#define lstat stat", and lstat.c is a no-op. AC_CHECK_FUNCS_ONCE([lstat]) if test $ac_cv_func_lstat = yes; then AC_REQUIRE([gl_FUNC_LSTAT_FOLLOWS_SLASHED_SYMLINK]) case $host_os,$gl_cv_func_lstat_dereferences_slashed_symlink in solaris* | *no) REPLACE_LSTAT=1 ;; esac else HAVE_LSTAT=0 fi ]) # Prerequisites of lib/lstat.c. AC_DEFUN([gl_PREREQ_LSTAT], [:]) AC_DEFUN([gl_FUNC_LSTAT_FOLLOWS_SLASHED_SYMLINK], [ dnl We don't use AC_FUNC_LSTAT_FOLLOWS_SLASHED_SYMLINK any more, because it dnl is no longer maintained in Autoconf and because it invokes AC_LIBOBJ. AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether lstat correctly handles trailing slash], [gl_cv_func_lstat_dereferences_slashed_symlink], [rm -f conftest.sym conftest.file echo >conftest.file AC_RUN_IFELSE( [AC_LANG_PROGRAM( [AC_INCLUDES_DEFAULT], [[struct stat sbuf; if (symlink ("conftest.file", "conftest.sym") != 0) return 1; /* Linux will dereference the symlink and fail, as required by POSIX. That is better in the sense that it means we will not have to compile and use the lstat wrapper. */ return lstat ("conftest.sym/", &sbuf) == 0; ]])], [gl_cv_func_lstat_dereferences_slashed_symlink=yes], [gl_cv_func_lstat_dereferences_slashed_symlink=no], [case "$host_os" in *-gnu*) # Guess yes on glibc systems. gl_cv_func_lstat_dereferences_slashed_symlink="guessing yes" ;; mingw*) # Guess no on native Windows. gl_cv_func_lstat_dereferences_slashed_symlink="guessing no" ;; *) # If we don't know, assume the worst. gl_cv_func_lstat_dereferences_slashed_symlink="guessing no" ;; esac ]) rm -f conftest.sym conftest.file ]) case "$gl_cv_func_lstat_dereferences_slashed_symlink" in *yes) AC_DEFINE_UNQUOTED([LSTAT_FOLLOWS_SLASHED_SYMLINK], [1], [Define to 1 if 'lstat' dereferences a symlink specified with a trailing slash.]) ;; esac ]) gnuastro-0.5/bootstrapped/m4/longlong.m40000644000175000017500000001120313217200022015232 00000000000000# longlong.m4 serial 17 dnl Copyright (C) 1999-2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # Define HAVE_LONG_LONG_INT if 'long long int' works. # This fixes a bug in Autoconf 2.61, and can be faster # than what's in Autoconf 2.62 through 2.68. # Note: If the type 'long long int' exists but is only 32 bits large # (as on some very old compilers), HAVE_LONG_LONG_INT will not be # defined. In this case you can treat 'long long int' like 'long int'. AC_DEFUN([AC_TYPE_LONG_LONG_INT], [ AC_REQUIRE([AC_TYPE_UNSIGNED_LONG_LONG_INT]) AC_CACHE_CHECK([for long long int], [ac_cv_type_long_long_int], [ac_cv_type_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then ac_cv_type_long_long_int=$ac_cv_type_unsigned_long_long_int if test $ac_cv_type_long_long_int = yes; then dnl Catch a bug in Tandem NonStop Kernel (OSS) cc -O circa 2004. dnl If cross compiling, assume the bug is not important, since dnl nobody cross compiles for this platform as far as we know. AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[@%:@include @%:@ifndef LLONG_MAX @%:@ define HALF \ (1LL << (sizeof (long long int) * CHAR_BIT - 2)) @%:@ define LLONG_MAX (HALF - 1 + HALF) @%:@endif]], [[long long int n = 1; int i; for (i = 0; ; i++) { long long int m = n << i; if (m >> i != n) return 1; if (LLONG_MAX / 2 < m) break; } return 0;]])], [], [ac_cv_type_long_long_int=no], [:]) fi fi]) if test $ac_cv_type_long_long_int = yes; then AC_DEFINE([HAVE_LONG_LONG_INT], [1], [Define to 1 if the system has the type 'long long int'.]) fi ]) # Define HAVE_UNSIGNED_LONG_LONG_INT if 'unsigned long long int' works. # This fixes a bug in Autoconf 2.61, and can be faster # than what's in Autoconf 2.62 through 2.68. # Note: If the type 'unsigned long long int' exists but is only 32 bits # large (as on some very old compilers), AC_TYPE_UNSIGNED_LONG_LONG_INT # will not be defined. In this case you can treat 'unsigned long long int' # like 'unsigned long int'. AC_DEFUN([AC_TYPE_UNSIGNED_LONG_LONG_INT], [ AC_CACHE_CHECK([for unsigned long long int], [ac_cv_type_unsigned_long_long_int], [ac_cv_type_unsigned_long_long_int=yes if test "x${ac_cv_prog_cc_c99-no}" = xno; then AC_LINK_IFELSE( [_AC_TYPE_LONG_LONG_SNIPPET], [], [ac_cv_type_unsigned_long_long_int=no]) fi]) if test $ac_cv_type_unsigned_long_long_int = yes; then AC_DEFINE([HAVE_UNSIGNED_LONG_LONG_INT], [1], [Define to 1 if the system has the type 'unsigned long long int'.]) fi ]) # Expands to a C program that can be used to test for simultaneous support # of 'long long' and 'unsigned long long'. We don't want to say that # 'long long' is available if 'unsigned long long' is not, or vice versa, # because too many programs rely on the symmetry between signed and unsigned # integer types (excluding 'bool'). AC_DEFUN([_AC_TYPE_LONG_LONG_SNIPPET], [ AC_LANG_PROGRAM( [[/* For now, do not test the preprocessor; as of 2007 there are too many implementations with broken preprocessors. Perhaps this can be revisited in 2012. In the meantime, code should not expect #if to work with literals wider than 32 bits. */ /* Test literals. */ long long int ll = 9223372036854775807ll; long long int nll = -9223372036854775807LL; unsigned long long int ull = 18446744073709551615ULL; /* Test constant expressions. */ typedef int a[((-9223372036854775807LL < 0 && 0 < 9223372036854775807ll) ? 1 : -1)]; typedef int b[(18446744073709551615ULL <= (unsigned long long int) -1 ? 1 : -1)]; int i = 63;]], [[/* Test availability of runtime routines for shift and division. */ long long int llmax = 9223372036854775807ll; unsigned long long int ullmax = 18446744073709551615ull; return ((ll << 63) | (ll >> 63) | (ll < i) | (ll > i) | (llmax / ll) | (llmax % ll) | (ull << 63) | (ull >> 63) | (ull << i) | (ull >> i) | (ullmax / ull) | (ullmax % ull));]]) ]) gnuastro-0.5/bootstrapped/m4/lock.m40000644000175000017500000000303713217200022014351 00000000000000# lock.m4 serial 14 dnl Copyright (C) 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_DEFUN([gl_LOCK], [ AC_REQUIRE([gl_THREADLIB]) if test "$gl_threads_api" = posix; then # OSF/1 4.0 and Mac OS X 10.1 lack the pthread_rwlock_t type and the # pthread_rwlock_* functions. has_rwlock=false AC_CHECK_TYPE([pthread_rwlock_t], [has_rwlock=true AC_DEFINE([HAVE_PTHREAD_RWLOCK], [1], [Define if the POSIX multithreading library has read/write locks.])], [], [#include ]) if $has_rwlock; then gl_PTHREAD_RWLOCK_RDLOCK_PREFER_WRITER fi # glibc defines PTHREAD_MUTEX_RECURSIVE as enum, not as a macro. AC_COMPILE_IFELSE([ AC_LANG_PROGRAM( [[#include ]], [[ #if __FreeBSD__ == 4 error "No, in FreeBSD 4.0 recursive mutexes actually don't work." #elif (defined __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ \ && __ENVIRONMENT_MAC_OS_X_VERSION_MIN_REQUIRED__ < 1070) error "No, in Mac OS X < 10.7 recursive mutexes actually don't work." #else int x = (int)PTHREAD_MUTEX_RECURSIVE; return !x; #endif ]])], [AC_DEFINE([HAVE_PTHREAD_MUTEX_RECURSIVE], [1], [Define if the defines PTHREAD_MUTEX_RECURSIVE.])]) fi gl_PREREQ_LOCK ]) # Prerequisites of lib/glthread/lock.c. AC_DEFUN([gl_PREREQ_LOCK], [:]) gnuastro-0.5/bootstrapped/m4/localtime-buffer.m40000644000175000017500000000123013217200022016632 00000000000000# localtime-buffer.m4 serial 1 dnl Copyright (C) 2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALTIME_BUFFER_DEFAULTS], [ NEED_LOCALTIME_BUFFER=0 ]) dnl Macro invoked from other modules, to signal that the compilation of dnl module 'localtime-buffer' is needed. AC_DEFUN([gl_LOCALTIME_BUFFER_NEEDED], [ AC_REQUIRE([gl_LOCALTIME_BUFFER_DEFAULTS]) AC_REQUIRE([gl_HEADER_TIME_H_DEFAULTS]) NEED_LOCALTIME_BUFFER=1 REPLACE_GMTIME=1 REPLACE_LOCALTIME=1 ]) gnuastro-0.5/bootstrapped/m4/localename.m40000644000175000017500000000113413217200022015515 00000000000000# localename.m4 serial 2 dnl Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALENAME], [ AC_REQUIRE([gt_LC_MESSAGES]) AC_REQUIRE([gt_INTL_MACOSX]) AC_CHECK_FUNCS([setlocale uselocale]) dnl Solaris 12 provides getlocalename_l, while Illumos doesn't have dnl it nor the equivalent. if test $ac_cv_func_uselocale = yes; then AC_CHECK_FUNCS([getlocalename_l]) fi ]) gnuastro-0.5/bootstrapped/m4/localeconv.m40000644000175000017500000000114713217200022015546 00000000000000# localeconv.m4 serial 1 dnl Copyright (C) 2012-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_LOCALECONV], [ AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) AC_REQUIRE([gl_LOCALE_H]) if test $REPLACE_STRUCT_LCONV = 1; then REPLACE_LOCALECONV=1 fi ]) # Prerequisites of lib/localeconv.c. AC_DEFUN([gl_PREREQ_LOCALECONV], [ AC_CHECK_MEMBERS([struct lconv.decimal_point], [], [], [[#include ]]) ]) gnuastro-0.5/bootstrapped/m4/locale_h.m40000644000175000017500000001037313217200022015170 00000000000000# locale_h.m4 serial 20 dnl Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALE_H], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) dnl Persuade glibc to define locale_t and the int_p_*, int_n_* dnl members of 'struct lconv'. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) dnl If is replaced, then must also be replaced. AC_REQUIRE([gl_STDDEF_H]) dnl Solaris 11.0 defines the int_p_*, int_n_* members of 'struct lconv' dnl only if _LCONV_C99 is defined. AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in solaris*) AC_DEFINE([_LCONV_C99], [1], [Define to 1 on Solaris.]) ;; esac AC_CACHE_CHECK([whether locale.h conforms to POSIX:2001], [gl_cv_header_locale_h_posix2001], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int x = LC_MESSAGES; int y = sizeof (((struct lconv *) 0)->decimal_point);]], [[]])], [gl_cv_header_locale_h_posix2001=yes], [gl_cv_header_locale_h_posix2001=no])]) dnl Check for . AC_CHECK_HEADERS_ONCE([xlocale.h]) if test $ac_cv_header_xlocale_h = yes; then HAVE_XLOCALE_H=1 dnl Check whether use of locale_t requires inclusion of , dnl e.g. on Mac OS X 10.5. If does not define locale_t by dnl itself, we assume that will do so. AC_CACHE_CHECK([whether locale.h defines locale_t], [gl_cv_header_locale_has_locale_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include locale_t x;]], [[]])], [gl_cv_header_locale_has_locale_t=yes], [gl_cv_header_locale_has_locale_t=no]) ]) if test $gl_cv_header_locale_has_locale_t = yes; then gl_cv_header_locale_h_needs_xlocale_h=no else gl_cv_header_locale_h_needs_xlocale_h=yes fi else HAVE_XLOCALE_H=0 gl_cv_header_locale_h_needs_xlocale_h=no fi AC_SUBST([HAVE_XLOCALE_H]) dnl Check whether 'struct lconv' is complete. dnl Bionic libc's 'struct lconv' is just a dummy. dnl On OpenBSD 4.9, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 9, Cygwin 1.5.x, dnl mingw, MSVC 9, it lacks the int_p_* and int_n_* members. AC_CACHE_CHECK([whether struct lconv is properly defined], [gl_cv_sys_struct_lconv_ok], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include struct lconv l; int x = sizeof (l.decimal_point); int y = sizeof (l.int_p_cs_precedes);]], [[]])], [gl_cv_sys_struct_lconv_ok=yes], [gl_cv_sys_struct_lconv_ok=no]) ]) if test $gl_cv_sys_struct_lconv_ok = no; then REPLACE_STRUCT_LCONV=1 fi dnl is always overridden, because of GNULIB_POSIXCHECK. gl_NEXT_HEADERS([locale.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include /* Some systems provide declarations in a non-standard header. */ #if HAVE_XLOCALE_H # include #endif ]], [setlocale duplocale]) ]) AC_DEFUN([gl_LOCALE_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_LOCALE_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_LOCALE_H_DEFAULTS], [ GNULIB_LOCALECONV=0; AC_SUBST([GNULIB_LOCALECONV]) GNULIB_SETLOCALE=0; AC_SUBST([GNULIB_SETLOCALE]) GNULIB_DUPLOCALE=0; AC_SUBST([GNULIB_DUPLOCALE]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DUPLOCALE=1; AC_SUBST([HAVE_DUPLOCALE]) REPLACE_LOCALECONV=0; AC_SUBST([REPLACE_LOCALECONV]) REPLACE_SETLOCALE=0; AC_SUBST([REPLACE_SETLOCALE]) REPLACE_DUPLOCALE=0; AC_SUBST([REPLACE_DUPLOCALE]) REPLACE_STRUCT_LCONV=0; AC_SUBST([REPLACE_STRUCT_LCONV]) ]) gnuastro-0.5/bootstrapped/m4/locale-zh.m40000644000175000017500000001270513217200022015301 00000000000000# locale-zh.m4 serial 13 dnl Copyright (C) 2003, 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a chinese locale with GB18030 encoding. AC_DEFUN([gt_LOCALE_ZH_CN], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a transitional chinese locale], [gt_cv_locale_zh_CN], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } /* Check whether a typical GB18030 multibyte sequence is recognized as a single wide character. This excludes the GB2312 and GBK encodings. */ if (mblen ("\203\062\332\066", 5) != 4) return 1; return 0; #endif } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Chinese_China.54936 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=Chinese_China.54936 else # None found. gt_cv_locale_zh_CN=none fi ;; solaris2.8) # On Solaris 8, the locales zh_CN.GB18030, zh_CN.GBK, zh.GBK are # broken. One witness is the test case in gl_MBRTOWC_SANITYCHECK. # Another witness is that "LC_ALL=zh_CN.GB18030 bash -c true" dumps core. gt_cv_locale_zh_CN=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the locale name without encoding suffix. if (LC_ALL=zh_CN LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN else # Test for the locale name with explicit encoding suffix. if (LC_ALL=zh_CN.GB18030 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_zh_CN=zh_CN.GB18030 else # None found. gt_cv_locale_zh_CN=none fi fi ;; esac else # If there was a link error, due to mblen(), the system is so old that # it certainly doesn't have a chinese locale. gt_cv_locale_zh_CN=none fi rm -fr conftest* ]) LOCALE_ZH_CN=$gt_cv_locale_zh_CN AC_SUBST([LOCALE_ZH_CN]) ]) gnuastro-0.5/bootstrapped/m4/locale-tr.m40000644000175000017500000001211113217200022015274 00000000000000# locale-tr.m4 serial 10 dnl Copyright (C) 2003, 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a turkish locale with UTF-8 encoding. AC_DEFUN([gt_LOCALE_TR_UTF8], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a turkish Unicode locale], [gt_cv_locale_tr_utf8], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. But BeOS does not implement the Turkish upper-/lowercase mappings. Therefore, let this program return 1 on BeOS. */ /* Check whether the given locale name is recognized by the system. */ #if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; #else if (setlocale (LC_ALL, "") == NULL) return 1; #endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the tr_TR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ #if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } #endif #ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; #endif /* Check whether in the abbreviation of the eighth month, the second character (should be U+011F: LATIN SMALL LETTER G WITH BREVE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1992 - 1900; t.tm_mon = 8 - 1; t.tm_mday = 19; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc4 || buf[2] != (char) 0x9f) return 1; /* Check whether the upper-/lowercase mappings are as expected for Turkish. */ if (towupper ('i') != 0x0130 || towlower (0x0130) != 'i' || towupper(0x0131) != 'I' || towlower ('I') != 0x0131) return 1; return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=Turkish_Turkey.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=Turkish_Turkey.65001 else # None found. gt_cv_locale_tr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=tr_TR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=tr_TR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=tr_TR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=tr_TR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=tr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_tr_utf8=tr.UTF-8 else # None found. gt_cv_locale_tr_utf8=none fi fi fi ;; esac else gt_cv_locale_tr_utf8=none fi rm -fr conftest* ]) LOCALE_TR_UTF8=$gt_cv_locale_tr_utf8 AC_SUBST([LOCALE_TR_UTF8]) ]) gnuastro-0.5/bootstrapped/m4/locale-ja.m40000644000175000017500000001326213217200022015251 00000000000000# locale-ja.m4 serial 13 dnl Copyright (C) 2003, 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a japanese locale with EUC-JP encoding. AC_DEFUN([gt_LOCALE_JA], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a traditional japanese locale], [gt_cv_locale_ja], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether MB_CUR_MAX is > 1. This excludes the dysfunctional locales on Cygwin 1.5.x. */ if (MB_CUR_MAX == 1) return 1; /* Check whether in a month name, no byte in the range 0x80..0x9F occurs. This excludes the UTF-8 encoding (except on MirBSD). */ { const char *p; t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%B", &t) < 2) return 1; for (p = buf; *p != '\0'; p++) if ((unsigned char) *p >= 0x80 && (unsigned char) *p < 0xa0) return 1; } return 0; #endif } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Note that on native Windows, the Japanese locale is # Japanese_Japan.932, and CP932 is very different from EUC-JP, so we # cannot use it here. gt_cv_locale_ja=none ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the AIX locale name. if (LC_ALL=ja_JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP else # Test for the locale name with explicit encoding suffix. if (LC_ALL=ja_JP.EUC-JP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC-JP else # Test for the HP-UX, OSF/1, NetBSD locale name. if (LC_ALL=ja_JP.eucJP LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.eucJP else # Test for the IRIX, FreeBSD locale name. if (LC_ALL=ja_JP.EUC LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja_JP.EUC else # Test for the Solaris 7 locale name. if (LC_ALL=ja LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_ja=ja else # Special test for NetBSD 1.6. if test -f /usr/share/locale/ja_JP.eucJP/LC_CTYPE; then gt_cv_locale_ja=ja_JP.eucJP else # None found. gt_cv_locale_ja=none fi fi fi fi fi fi ;; esac fi rm -fr conftest* ]) LOCALE_JA=$gt_cv_locale_ja AC_SUBST([LOCALE_JA]) ]) gnuastro-0.5/bootstrapped/m4/locale-fr.m40000644000175000017500000002466213217200022015274 00000000000000# locale-fr.m4 serial 18 dnl Copyright (C) 2003, 2005-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. dnl Determine the name of a french locale with traditional encoding. AC_DEFUN([gt_LOCALE_FR], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a traditional french locale], [gt_cv_locale_fr], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if defined __BEOS__ || defined __HAIKU__ return 1; #else /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. On MirBSD 10, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "UTF-8". */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0 || strcmp (cs, "UTF-8") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is only one byte long. This excludes the UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 3 || buf[2] != 'v') return 1; # if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; # endif return 0; #endif } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the native Windows locale name. if (LC_ALL=French_France.1252 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=French_France.1252 else # None found. gt_cv_locale_fr=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.ISO-8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO-8859-1 else # Test for the AIX, OSF/1, FreeBSD, NetBSD, OpenBSD locale name. if (LC_ALL=fr_FR.ISO8859-1 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.ISO8859-1 else # Test for the HP-UX locale name. if (LC_ALL=fr_FR.iso88591 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr_FR.iso88591 else # Test for the Solaris 7 locale name. if (LC_ALL=fr LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr=fr else # None found. gt_cv_locale_fr=none fi fi fi fi fi ;; esac fi rm -fr conftest* ]) LOCALE_FR=$gt_cv_locale_fr AC_SUBST([LOCALE_FR]) ]) dnl Determine the name of a french locale with UTF-8 encoding. AC_DEFUN([gt_LOCALE_FR_UTF8], [ AC_REQUIRE([AM_LANGINFO_CODESET]) AC_CACHE_CHECK([for a french Unicode locale], [gt_cv_locale_fr_utf8], [ AC_LANG_CONFTEST([AC_LANG_SOURCE([ changequote(,)dnl #include #include #if HAVE_LANGINFO_CODESET # include #endif #include #include struct tm t; char buf[16]; int main () { /* On BeOS and Haiku, locales are not implemented in libc. Rather, libintl imitates locale dependent behaviour by looking at the environment variables, and all locales use the UTF-8 encoding. */ #if !(defined __BEOS__ || defined __HAIKU__) /* Check whether the given locale name is recognized by the system. */ # if (defined _WIN32 || defined __WIN32__) && !defined __CYGWIN__ /* On native Windows, setlocale(category, "") looks at the system settings, not at the environment variables. Also, when an encoding suffix such as ".65001" or ".54936" is specified, it succeeds but sets the LC_CTYPE category of the locale to "C". */ if (setlocale (LC_ALL, getenv ("LC_ALL")) == NULL || strcmp (setlocale (LC_CTYPE, NULL), "C") == 0) return 1; # else if (setlocale (LC_ALL, "") == NULL) return 1; # endif /* Check whether nl_langinfo(CODESET) is nonempty and not "ASCII" or "646". On Mac OS X 10.3.5 (Darwin 7.5) in the fr_FR locale, nl_langinfo(CODESET) is empty, and the behaviour of Tcl 8.4 in this locale is not useful. On OpenBSD 4.0, when an unsupported locale is specified, setlocale() succeeds but then nl_langinfo(CODESET) is "646". In this situation, some unit tests fail. */ # if HAVE_LANGINFO_CODESET { const char *cs = nl_langinfo (CODESET); if (cs[0] == '\0' || strcmp (cs, "ASCII") == 0 || strcmp (cs, "646") == 0) return 1; } # endif # ifdef __CYGWIN__ /* On Cygwin, avoid locale names without encoding suffix, because the locale_charset() function relies on the encoding suffix. Note that LC_ALL is set on the command line. */ if (strchr (getenv ("LC_ALL"), '.') == NULL) return 1; # endif /* Check whether in the abbreviation of the second month, the second character (should be U+00E9: LATIN SMALL LETTER E WITH ACUTE) is two bytes long, with UTF-8 encoding. */ t.tm_year = 1975 - 1900; t.tm_mon = 2 - 1; t.tm_mday = 4; if (strftime (buf, sizeof (buf), "%b", &t) < 4 || buf[1] != (char) 0xc3 || buf[2] != (char) 0xa9 || buf[3] != 'v') return 1; #endif #if !defined __BIONIC__ /* Bionic libc's 'struct lconv' is just a dummy. */ /* Check whether the decimal separator is a comma. On NetBSD 3.0 in the fr_FR.ISO8859-1 locale, localeconv()->decimal_point are nl_langinfo(RADIXCHAR) are both ".". */ if (localeconv () ->decimal_point[0] != ',') return 1; #endif return 0; } changequote([,])dnl ])]) if AC_TRY_EVAL([ac_link]) && test -s conftest$ac_exeext; then case "$host_os" in # Handle native Windows specially, because there setlocale() interprets # "ar" as "Arabic" or "Arabic_Saudi Arabia.1256", # "fr" or "fra" as "French" or "French_France.1252", # "ge"(!) or "deu"(!) as "German" or "German_Germany.1252", # "ja" as "Japanese" or "Japanese_Japan.932", # and similar. mingw*) # Test for the hypothetical native Windows locale name. if (LC_ALL=French_France.65001 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=French_France.65001 else # None found. gt_cv_locale_fr_utf8=none fi ;; *) # Setting LC_ALL is not enough. Need to set LC_TIME to empty, because # otherwise on Mac OS X 10.3.5 the LC_TIME=C from the beginning of the # configure script would override the LC_ALL setting. Likewise for # LC_CTYPE, which is also set at the beginning of the configure script. # Test for the usual locale name. if (LC_ALL=fr_FR LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR else # Test for the locale name with explicit encoding suffix. if (LC_ALL=fr_FR.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr_FR.UTF-8 else # Test for the Solaris 7 locale name. if (LC_ALL=fr.UTF-8 LC_TIME= LC_CTYPE= ./conftest; exit) 2>/dev/null; then gt_cv_locale_fr_utf8=fr.UTF-8 else # None found. gt_cv_locale_fr_utf8=none fi fi fi ;; esac fi rm -fr conftest* ]) LOCALE_FR_UTF8=$gt_cv_locale_fr_utf8 AC_SUBST([LOCALE_FR_UTF8]) ]) gnuastro-0.5/bootstrapped/m4/localcharset.m40000644000175000017500000000112513217200022016061 00000000000000# localcharset.m4 serial 7 dnl Copyright (C) 2002, 2004, 2006, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LOCALCHARSET], [ dnl Prerequisites of lib/localcharset.c. AC_REQUIRE([AM_LANGINFO_CODESET]) AC_REQUIRE([gl_FCNTL_O_FLAGS]) AC_CHECK_DECLS_ONCE([getc_unlocked]) dnl Prerequisites of the lib/Makefile.am snippet. AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_GLIBC21]) ]) gnuastro-0.5/bootstrapped/m4/limits-h.m40000644000175000017500000000202613217200022015144 00000000000000dnl Check whether limits.h has needed features. dnl Copyright 2016-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. AC_DEFUN_ONCE([gl_LIMITS_H], [ gl_CHECK_NEXT_HEADERS([limits.h]) AC_CACHE_CHECK([whether limits.h has ULLONG_WIDTH etc.], [gl_cv_header_limits_width], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#ifndef __STDC_WANT_IEC_60559_BFP_EXT__ #define __STDC_WANT_IEC_60559_BFP_EXT__ 1 #endif #include int ullw = ULLONG_WIDTH;]])], [gl_cv_header_limits_width=yes], [gl_cv_header_limits_width=no])]) if test "$gl_cv_header_limits_width" = yes; then LIMITS_H= else LIMITS_H=limits.h fi AC_SUBST([LIMITS_H]) AM_CONDITIONAL([GL_GENERATE_LIMITS_H], [test -n "$LIMITS_H"]) ]) gnuastro-0.5/bootstrapped/m4/libunistring-base.m40000644000175000017500000001426013217200022017042 00000000000000# libunistring-base.m4 serial 5 dnl Copyright (C) 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paolo Bonzini and Bruno Haible. dnl gl_LIBUNISTRING_MODULE([VERSION], [Module]) dnl Declares that the source files of Module should be compiled, unless we dnl are linking with libunistring and its version is >= the given VERSION. dnl Defines an automake conditional LIBUNISTRING_COMPILE_$MODULE that is dnl true if the source files of Module should be compiled. dnl This macro is to be used for public libunistring API, not for dnl undocumented API. dnl dnl You have to bump the VERSION argument to the next projected version dnl number each time you make a change that affects the behaviour of the dnl functions defined in Module (even if the sources of Module itself do not dnl change). AC_DEFUN([gl_LIBUNISTRING_MODULE], [ AC_REQUIRE([gl_LIBUNISTRING_LIB_PREPARE]) dnl Use the variables HAVE_LIBUNISTRING, LIBUNISTRING_VERSION from dnl gl_LIBUNISTRING_CORE if that macro has been run. AM_CONDITIONAL(AS_TR_CPP([LIBUNISTRING_COMPILE_$2]), [gl_LIBUNISTRING_VERSION_CMP([$1])]) ]) dnl gl_LIBUNISTRING_LIBHEADER([VERSION], [HeaderFile]) dnl Declares that HeaderFile should be created, unless we are linking dnl with libunistring and its version is >= the given VERSION. dnl HeaderFile should be relative to the lib directory and end in '.h'. dnl Prepares for substituting LIBUNISTRING_HEADERFILE (to HeaderFile or empty). dnl dnl When we are linking with the already installed libunistring and its version dnl is < VERSION, we create HeaderFile here, because we may compile functions dnl (via gl_LIBUNISTRING_MODULE above) that are not contained in the installed dnl version. dnl When we are linking with the already installed libunistring and its version dnl is > VERSION, we don't create HeaderFile here: it could cause compilation dnl errors in other libunistring header files if some types are missing. dnl dnl You have to bump the VERSION argument to the next projected version dnl number each time you make a non-comment change to the HeaderFile. AC_DEFUN([gl_LIBUNISTRING_LIBHEADER], [ AC_REQUIRE([gl_LIBUNISTRING_LIB_PREPARE]) dnl Use the variables HAVE_LIBUNISTRING, LIBUNISTRING_VERSION from dnl gl_LIBUNISTRING_CORE if that macro has been run. if gl_LIBUNISTRING_VERSION_CMP([$1]); then LIBUNISTRING_[]AS_TR_CPP([$2])='$2' else LIBUNISTRING_[]AS_TR_CPP([$2])= fi AC_SUBST([LIBUNISTRING_]AS_TR_CPP([$2])) ]) dnl Miscellaneous preparations/initializations. AC_DEFUN([gl_LIBUNISTRING_LIB_PREPARE], [ dnl Ensure that HAVE_LIBUNISTRING is fully determined at this point. m4_ifdef([gl_LIBUNISTRING], [AC_REQUIRE([gl_LIBUNISTRING])]) AC_REQUIRE([AC_PROG_AWK]) dnl Sed expressions to extract the parts of a version number. changequote(,) gl_libunistring_sed_extract_major='/^[0-9]/{s/^\([0-9]*\).*/\1/p;q;} i\ 0 q ' gl_libunistring_sed_extract_minor='/^[0-9][0-9]*[.][0-9]/{s/^[0-9]*[.]\([0-9]*\).*/\1/p;q;} i\ 0 q ' gl_libunistring_sed_extract_subminor='/^[0-9][0-9]*[.][0-9][0-9]*[.][0-9]/{s/^[0-9]*[.][0-9]*[.]\([0-9]*\).*/\1/p;q;} i\ 0 q ' changequote([,]) if test "$HAVE_LIBUNISTRING" = yes; then LIBUNISTRING_VERSION_MAJOR=`echo "$LIBUNISTRING_VERSION" | sed -n -e "$gl_libunistring_sed_extract_major"` LIBUNISTRING_VERSION_MINOR=`echo "$LIBUNISTRING_VERSION" | sed -n -e "$gl_libunistring_sed_extract_minor"` LIBUNISTRING_VERSION_SUBMINOR=`echo "$LIBUNISTRING_VERSION" | sed -n -e "$gl_libunistring_sed_extract_subminor"` fi ]) dnl gl_LIBUNISTRING_VERSION_CMP([VERSION]) dnl Expands to a shell statement that evaluates to true if LIBUNISTRING_VERSION dnl is less than the VERSION argument. AC_DEFUN([gl_LIBUNISTRING_VERSION_CMP], [ { test "$HAVE_LIBUNISTRING" != yes \ || { dnl AS_LITERAL_IF exists and works fine since autoconf-2.59 at least. AS_LITERAL_IF([$1], [dnl This is the optimized variant, that assumes the argument is a literal: m4_pushdef([requested_version_major], [gl_LIBUNISTRING_ARG_OR_ZERO(m4_bpatsubst([$1], [^\([0-9]*\).*], [\1]), [])]) m4_pushdef([requested_version_minor], [gl_LIBUNISTRING_ARG_OR_ZERO(m4_bpatsubst([$1], [^[0-9]*[.]\([0-9]*\).*], [\1]), [$1])]) m4_pushdef([requested_version_subminor], [gl_LIBUNISTRING_ARG_OR_ZERO(m4_bpatsubst([$1], [^[0-9]*[.][0-9]*[.]\([0-9]*\).*], [\1]), [$1])]) test $LIBUNISTRING_VERSION_MAJOR -lt requested_version_major \ || { test $LIBUNISTRING_VERSION_MAJOR -eq requested_version_major \ && { test $LIBUNISTRING_VERSION_MINOR -lt requested_version_minor \ || { test $LIBUNISTRING_VERSION_MINOR -eq requested_version_minor \ && test $LIBUNISTRING_VERSION_SUBMINOR -lt requested_version_subminor } } } m4_popdef([requested_version_subminor]) m4_popdef([requested_version_minor]) m4_popdef([requested_version_major]) ], [dnl This is the unoptimized variant: requested_version_major=`echo '$1' | sed -n -e "$gl_libunistring_sed_extract_major"` requested_version_minor=`echo '$1' | sed -n -e "$gl_libunistring_sed_extract_minor"` requested_version_subminor=`echo '$1' | sed -n -e "$gl_libunistring_sed_extract_subminor"` test $LIBUNISTRING_VERSION_MAJOR -lt $requested_version_major \ || { test $LIBUNISTRING_VERSION_MAJOR -eq $requested_version_major \ && { test $LIBUNISTRING_VERSION_MINOR -lt $requested_version_minor \ || { test $LIBUNISTRING_VERSION_MINOR -eq $requested_version_minor \ && test $LIBUNISTRING_VERSION_SUBMINOR -lt $requested_version_subminor } } } ]) } }]) dnl gl_LIBUNISTRING_ARG_OR_ZERO([ARG], [ORIG]) expands to ARG if it is not the dnl same as ORIG, otherwise to 0. m4_define([gl_LIBUNISTRING_ARG_OR_ZERO], [m4_if([$1], [$2], [0], [$1])]) gnuastro-0.5/bootstrapped/m4/libtool.m40000644000175000017500000112707613217177774015133 00000000000000# libtool.m4 - Configure libtool for the host system. -*-Autoconf-*- # # Copyright (C) 1996-2001, 2003-2017 Free Software Foundation, Inc. # Written by Gordon Matzigkeit, 1996 # # This file is free software; the Free Software Foundation gives # unlimited permission to copy and/or distribute it, with or without # modifications, as long as this notice is preserved. m4_define([_LT_COPYING], [dnl # Copyright (C) 2014 Free Software Foundation, Inc. # This is free software; see the source for copying conditions. There is NO # warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. # GNU Libtool is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2 of of the License, or # (at your option) any later version. # # As a special exception to the GNU General Public License, if you # distribute this file as part of a program or library that is built # using GNU Libtool, you may include this file under the same # distribution terms that you use for the rest of that program. # # GNU Libtool is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . ]) # serial 58 LT_INIT # LT_PREREQ(VERSION) # ------------------ # Complain and exit if this libtool version is less that VERSION. m4_defun([LT_PREREQ], [m4_if(m4_version_compare(m4_defn([LT_PACKAGE_VERSION]), [$1]), -1, [m4_default([$3], [m4_fatal([Libtool version $1 or higher is required], 63)])], [$2])]) # _LT_CHECK_BUILDDIR # ------------------ # Complain if the absolute build directory name contains unusual characters m4_defun([_LT_CHECK_BUILDDIR], [case `pwd` in *\ * | *\ *) AC_MSG_WARN([Libtool does not cope well with whitespace in `pwd`]) ;; esac ]) # LT_INIT([OPTIONS]) # ------------------ AC_DEFUN([LT_INIT], [AC_PREREQ([2.62])dnl We use AC_PATH_PROGS_FEATURE_CHECK AC_REQUIRE([AC_CONFIG_AUX_DIR_DEFAULT])dnl AC_BEFORE([$0], [LT_LANG])dnl AC_BEFORE([$0], [LT_OUTPUT])dnl AC_BEFORE([$0], [LTDL_INIT])dnl m4_require([_LT_CHECK_BUILDDIR])dnl dnl Autoconf doesn't catch unexpanded LT_ macros by default: m4_pattern_forbid([^_?LT_[A-Z_]+$])dnl m4_pattern_allow([^(_LT_EOF|LT_DLGLOBAL|LT_DLLAZY_OR_NOW|LT_MULTI_MODULE)$])dnl dnl aclocal doesn't pull ltoptions.m4, ltsugar.m4, or ltversion.m4 dnl unless we require an AC_DEFUNed macro: AC_REQUIRE([LTOPTIONS_VERSION])dnl AC_REQUIRE([LTSUGAR_VERSION])dnl AC_REQUIRE([LTVERSION_VERSION])dnl AC_REQUIRE([LTOBSOLETE_VERSION])dnl m4_require([_LT_PROG_LTMAIN])dnl _LT_SHELL_INIT([SHELL=${CONFIG_SHELL-/bin/sh}]) dnl Parse OPTIONS _LT_SET_OPTIONS([$0], [$1]) # This can be used to rebuild libtool when needed LIBTOOL_DEPS=$ltmain # Always use our own libtool. LIBTOOL='$(SHELL) $(top_builddir)/libtool' AC_SUBST(LIBTOOL)dnl _LT_SETUP # Only expand once: m4_define([LT_INIT]) ])# LT_INIT # Old names: AU_ALIAS([AC_PROG_LIBTOOL], [LT_INIT]) AU_ALIAS([AM_PROG_LIBTOOL], [LT_INIT]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_PROG_LIBTOOL], []) dnl AC_DEFUN([AM_PROG_LIBTOOL], []) # _LT_PREPARE_CC_BASENAME # ----------------------- m4_defun([_LT_PREPARE_CC_BASENAME], [ # Calculate cc_basename. Skip known compiler wrappers and cross-prefix. func_cc_basename () { for cc_temp in @S|@*""; do case $cc_temp in compile | *[[\\/]]compile | ccache | *[[\\/]]ccache ) ;; distcc | *[[\\/]]distcc | purify | *[[\\/]]purify ) ;; \-*) ;; *) break;; esac done func_cc_basename_result=`$ECHO "$cc_temp" | $SED "s%.*/%%; s%^$host_alias-%%"` } ])# _LT_PREPARE_CC_BASENAME # _LT_CC_BASENAME(CC) # ------------------- # It would be clearer to call AC_REQUIREs from _LT_PREPARE_CC_BASENAME, # but that macro is also expanded into generated libtool script, which # arranges for $SED and $ECHO to be set by different means. m4_defun([_LT_CC_BASENAME], [m4_require([_LT_PREPARE_CC_BASENAME])dnl AC_REQUIRE([_LT_DECL_SED])dnl AC_REQUIRE([_LT_PROG_ECHO_BACKSLASH])dnl func_cc_basename $1 cc_basename=$func_cc_basename_result ]) # _LT_FILEUTILS_DEFAULTS # ---------------------- # It is okay to use these file commands and assume they have been set # sensibly after 'm4_require([_LT_FILEUTILS_DEFAULTS])'. m4_defun([_LT_FILEUTILS_DEFAULTS], [: ${CP="cp -f"} : ${MV="mv -f"} : ${RM="rm -f"} ])# _LT_FILEUTILS_DEFAULTS # _LT_SETUP # --------- m4_defun([_LT_SETUP], [AC_REQUIRE([AC_CANONICAL_HOST])dnl AC_REQUIRE([AC_CANONICAL_BUILD])dnl AC_REQUIRE([_LT_PREPARE_SED_QUOTE_VARS])dnl AC_REQUIRE([_LT_PROG_ECHO_BACKSLASH])dnl _LT_DECL([], [PATH_SEPARATOR], [1], [The PATH separator for the build system])dnl dnl _LT_DECL([], [host_alias], [0], [The host system])dnl _LT_DECL([], [host], [0])dnl _LT_DECL([], [host_os], [0])dnl dnl _LT_DECL([], [build_alias], [0], [The build system])dnl _LT_DECL([], [build], [0])dnl _LT_DECL([], [build_os], [0])dnl dnl AC_REQUIRE([AC_PROG_CC])dnl AC_REQUIRE([LT_PATH_LD])dnl AC_REQUIRE([LT_PATH_NM])dnl dnl AC_REQUIRE([AC_PROG_LN_S])dnl test -z "$LN_S" && LN_S="ln -s" _LT_DECL([], [LN_S], [1], [Whether we need soft or hard links])dnl dnl AC_REQUIRE([LT_CMD_MAX_LEN])dnl _LT_DECL([objext], [ac_objext], [0], [Object file suffix (normally "o")])dnl _LT_DECL([], [exeext], [0], [Executable file suffix (normally "")])dnl dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_CHECK_SHELL_FEATURES])dnl m4_require([_LT_PATH_CONVERSION_FUNCTIONS])dnl m4_require([_LT_CMD_RELOAD])dnl m4_require([_LT_CHECK_MAGIC_METHOD])dnl m4_require([_LT_CHECK_SHAREDLIB_FROM_LINKLIB])dnl m4_require([_LT_CMD_OLD_ARCHIVE])dnl m4_require([_LT_CMD_GLOBAL_SYMBOLS])dnl m4_require([_LT_WITH_SYSROOT])dnl m4_require([_LT_CMD_TRUNCATE])dnl _LT_CONFIG_LIBTOOL_INIT([ # See if we are running on zsh, and set the options that allow our # commands through without removal of \ escapes INIT. if test -n "\${ZSH_VERSION+set}"; then setopt NO_GLOB_SUBST fi ]) if test -n "${ZSH_VERSION+set}"; then setopt NO_GLOB_SUBST fi _LT_CHECK_OBJDIR m4_require([_LT_TAG_COMPILER])dnl case $host_os in aix3*) # AIX sometimes has problems with the GCC collect2 program. For some # reason, if we set the COLLECT_NAMES environment variable, the problems # vanish in a puff of smoke. if test set != "${COLLECT_NAMES+set}"; then COLLECT_NAMES= export COLLECT_NAMES fi ;; esac # Global variables: ofile=libtool can_build_shared=yes # All known linkers require a '.a' archive for static linking (except MSVC, # which needs '.lib'). libext=a with_gnu_ld=$lt_cv_prog_gnu_ld old_CC=$CC old_CFLAGS=$CFLAGS # Set sane defaults for various variables test -z "$CC" && CC=cc test -z "$LTCC" && LTCC=$CC test -z "$LTCFLAGS" && LTCFLAGS=$CFLAGS test -z "$LD" && LD=ld test -z "$ac_objext" && ac_objext=o _LT_CC_BASENAME([$compiler]) # Only perform the check for file, if the check method requires it test -z "$MAGIC_CMD" && MAGIC_CMD=file case $deplibs_check_method in file_magic*) if test "$file_magic_cmd" = '$MAGIC_CMD'; then _LT_PATH_MAGIC fi ;; esac # Use C for the default configuration in the libtool script LT_SUPPORTED_TAG([CC]) _LT_LANG_C_CONFIG _LT_LANG_DEFAULT_CONFIG _LT_CONFIG_COMMANDS ])# _LT_SETUP # _LT_PREPARE_SED_QUOTE_VARS # -------------------------- # Define a few sed substitution that help us do robust quoting. m4_defun([_LT_PREPARE_SED_QUOTE_VARS], [# Backslashify metacharacters that are still active within # double-quoted strings. sed_quote_subst='s/\([["`$\\]]\)/\\\1/g' # Same as above, but do not quote variable references. double_quote_subst='s/\([["`\\]]\)/\\\1/g' # Sed substitution to delay expansion of an escaped shell variable in a # double_quote_subst'ed string. delay_variable_subst='s/\\\\\\\\\\\$/\\\\\\$/g' # Sed substitution to delay expansion of an escaped single quote. delay_single_quote_subst='s/'\''/'\'\\\\\\\'\''/g' # Sed substitution to avoid accidental globbing in evaled expressions no_glob_subst='s/\*/\\\*/g' ]) # _LT_PROG_LTMAIN # --------------- # Note that this code is called both from 'configure', and 'config.status' # now that we use AC_CONFIG_COMMANDS to generate libtool. 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Don't try to run-time override # by AR_FLAGS because that was never working and AR_FLAGS is about to die. _LT_DECL([], [AR_FLAGS], [\@S|@{ARFLAGS-"\@S|@lt_ar_flags"}], [Flags to create an archive]) AC_CACHE_CHECK([for archiver @FILE support], [lt_cv_ar_at_file], [lt_cv_ar_at_file=no AC_COMPILE_IFELSE([AC_LANG_PROGRAM], [echo conftest.$ac_objext > conftest.lst lt_ar_try='$AR $AR_FLAGS libconftest.a @conftest.lst >&AS_MESSAGE_LOG_FD' AC_TRY_EVAL([lt_ar_try]) if test 0 -eq "$ac_status"; then # Ensure the archiver fails upon bogus file names. rm -f conftest.$ac_objext libconftest.a AC_TRY_EVAL([lt_ar_try]) if test 0 -ne "$ac_status"; then lt_cv_ar_at_file=@ fi fi rm -f conftest.* libconftest.a ]) ]) if test no = "$lt_cv_ar_at_file"; then archiver_list_spec= else archiver_list_spec=$lt_cv_ar_at_file fi _LT_DECL([], [archiver_list_spec], [1], [How to feed a file listing to the archiver]) ])# _LT_PROG_AR # _LT_CMD_OLD_ARCHIVE # ------------------- m4_defun([_LT_CMD_OLD_ARCHIVE], [_LT_PROG_AR AC_CHECK_TOOL(STRIP, strip, :) test -z "$STRIP" && STRIP=: _LT_DECL([], [STRIP], [1], [A symbol stripping program]) AC_CHECK_TOOL(RANLIB, ranlib, :) test -z "$RANLIB" && RANLIB=: _LT_DECL([], [RANLIB], [1], [Commands used to install an old-style archive]) # Determine commands to create old-style static archives. old_archive_cmds='$AR $AR_FLAGS $oldlib$oldobjs' old_postinstall_cmds='chmod 644 $oldlib' old_postuninstall_cmds= if test -n "$RANLIB"; then case $host_os in bitrig* | openbsd*) old_postinstall_cmds="$old_postinstall_cmds~\$RANLIB -t \$tool_oldlib" ;; *) old_postinstall_cmds="$old_postinstall_cmds~\$RANLIB \$tool_oldlib" ;; esac old_archive_cmds="$old_archive_cmds~\$RANLIB \$tool_oldlib" fi case $host_os in darwin*) lock_old_archive_extraction=yes ;; *) lock_old_archive_extraction=no ;; esac _LT_DECL([], [old_postinstall_cmds], [2]) _LT_DECL([], [old_postuninstall_cmds], [2]) _LT_TAGDECL([], [old_archive_cmds], [2], [Commands used to build an old-style archive]) _LT_DECL([], [lock_old_archive_extraction], [0], [Whether to use a lock for old archive extraction]) ])# _LT_CMD_OLD_ARCHIVE # _LT_COMPILER_OPTION(MESSAGE, VARIABLE-NAME, FLAGS, # [OUTPUT-FILE], [ACTION-SUCCESS], [ACTION-FAILURE]) # ---------------------------------------------------------------- # Check whether the given compiler option works AC_DEFUN([_LT_COMPILER_OPTION], [m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_DECL_SED])dnl AC_CACHE_CHECK([$1], [$2], [$2=no m4_if([$4], , [ac_outfile=conftest.$ac_objext], [ac_outfile=$4]) echo "$lt_simple_compile_test_code" > conftest.$ac_ext lt_compiler_flag="$3" ## exclude from sc_useless_quotes_in_assignment # Insert the option either (1) after the last *FLAGS variable, or # (2) before a word containing "conftest.", or (3) at the end. # Note that $ac_compile itself does not contain backslashes and begins # with a dollar sign (not a hyphen), so the echo should work correctly. # The option is referenced via a variable to avoid confusing sed. lt_compile=`echo "$ac_compile" | $SED \ -e 's:.*FLAGS}\{0,1\} :&$lt_compiler_flag :; t' \ -e 's: [[^ ]]*conftest\.: $lt_compiler_flag&:; t' \ -e 's:$: $lt_compiler_flag:'` (eval echo "\"\$as_me:$LINENO: $lt_compile\"" >&AS_MESSAGE_LOG_FD) (eval "$lt_compile" 2>conftest.err) ac_status=$? cat conftest.err >&AS_MESSAGE_LOG_FD echo "$as_me:$LINENO: \$? = $ac_status" >&AS_MESSAGE_LOG_FD if (exit $ac_status) && test -s "$ac_outfile"; then # The compiler can only warn and ignore the option if not recognized # So say no if there are warnings other than the usual output. $ECHO "$_lt_compiler_boilerplate" | $SED '/^$/d' >conftest.exp $SED '/^$/d; /^ *+/d' conftest.err >conftest.er2 if test ! -s conftest.er2 || diff conftest.exp conftest.er2 >/dev/null; then $2=yes fi fi $RM conftest* ]) if test yes = "[$]$2"; then m4_if([$5], , :, [$5]) else m4_if([$6], , :, [$6]) fi ])# _LT_COMPILER_OPTION # Old name: AU_ALIAS([AC_LIBTOOL_COMPILER_OPTION], [_LT_COMPILER_OPTION]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_COMPILER_OPTION], []) # _LT_LINKER_OPTION(MESSAGE, VARIABLE-NAME, FLAGS, # [ACTION-SUCCESS], [ACTION-FAILURE]) # ---------------------------------------------------- # Check whether the given linker option works AC_DEFUN([_LT_LINKER_OPTION], [m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_DECL_SED])dnl AC_CACHE_CHECK([$1], [$2], [$2=no save_LDFLAGS=$LDFLAGS LDFLAGS="$LDFLAGS $3" echo "$lt_simple_link_test_code" > conftest.$ac_ext if (eval $ac_link 2>conftest.err) && test -s conftest$ac_exeext; then # The linker can only warn and ignore the option if not recognized # So say no if there are warnings if test -s conftest.err; then # Append any errors to the config.log. cat conftest.err 1>&AS_MESSAGE_LOG_FD $ECHO "$_lt_linker_boilerplate" | $SED '/^$/d' > conftest.exp $SED '/^$/d; /^ *+/d' conftest.err >conftest.er2 if diff conftest.exp conftest.er2 >/dev/null; then $2=yes fi else $2=yes fi fi $RM -r conftest* LDFLAGS=$save_LDFLAGS ]) if test yes = "[$]$2"; then m4_if([$4], , :, [$4]) else m4_if([$5], , :, [$5]) fi ])# _LT_LINKER_OPTION # Old name: AU_ALIAS([AC_LIBTOOL_LINKER_OPTION], [_LT_LINKER_OPTION]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_LINKER_OPTION], []) # LT_CMD_MAX_LEN #--------------- AC_DEFUN([LT_CMD_MAX_LEN], [AC_REQUIRE([AC_CANONICAL_HOST])dnl # find the maximum length of command line arguments AC_MSG_CHECKING([the maximum length of command line arguments]) AC_CACHE_VAL([lt_cv_sys_max_cmd_len], [dnl i=0 teststring=ABCD case $build_os in msdosdjgpp*) # On DJGPP, this test can blow up pretty badly due to problems in libc # (any single argument exceeding 2000 bytes causes a buffer overrun # during glob expansion). Even if it were fixed, the result of this # check would be larger than it should be. lt_cv_sys_max_cmd_len=12288; # 12K is about right ;; gnu*) # Under GNU Hurd, this test is not required because there is # no limit to the length of command line arguments. # Libtool will interpret -1 as no limit whatsoever lt_cv_sys_max_cmd_len=-1; ;; cygwin* | mingw* | cegcc*) # On Win9x/ME, this test blows up -- it succeeds, but takes # about 5 minutes as the teststring grows exponentially. # Worse, since 9x/ME are not pre-emptively multitasking, # you end up with a "frozen" computer, even though with patience # the test eventually succeeds (with a max line length of 256k). # Instead, let's just punt: use the minimum linelength reported by # all of the supported platforms: 8192 (on NT/2K/XP). lt_cv_sys_max_cmd_len=8192; ;; mint*) # On MiNT this can take a long time and run out of memory. lt_cv_sys_max_cmd_len=8192; ;; amigaos*) # On AmigaOS with pdksh, this test takes hours, literally. # So we just punt and use a minimum line length of 8192. lt_cv_sys_max_cmd_len=8192; ;; bitrig* | darwin* | dragonfly* | freebsd* | netbsd* | openbsd*) # This has been around since 386BSD, at least. Likely further. if test -x /sbin/sysctl; then lt_cv_sys_max_cmd_len=`/sbin/sysctl -n kern.argmax` elif test -x /usr/sbin/sysctl; then lt_cv_sys_max_cmd_len=`/usr/sbin/sysctl -n kern.argmax` else lt_cv_sys_max_cmd_len=65536 # usable default for all BSDs fi # And add a safety zone lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \/ 4` lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \* 3` ;; interix*) # We know the value 262144 and hardcode it with a safety zone (like BSD) lt_cv_sys_max_cmd_len=196608 ;; os2*) # The test takes a long time on OS/2. lt_cv_sys_max_cmd_len=8192 ;; osf*) # Dr. Hans Ekkehard Plesser reports seeing a kernel panic running configure # due to this test when exec_disable_arg_limit is 1 on Tru64. It is not # nice to cause kernel panics so lets avoid the loop below. # First set a reasonable default. lt_cv_sys_max_cmd_len=16384 # if test -x /sbin/sysconfig; then case `/sbin/sysconfig -q proc exec_disable_arg_limit` in *1*) lt_cv_sys_max_cmd_len=-1 ;; esac fi ;; sco3.2v5*) lt_cv_sys_max_cmd_len=102400 ;; sysv5* | sco5v6* | sysv4.2uw2*) kargmax=`grep ARG_MAX /etc/conf/cf.d/stune 2>/dev/null` if test -n "$kargmax"; then lt_cv_sys_max_cmd_len=`echo $kargmax | sed 's/.*[[ ]]//'` else lt_cv_sys_max_cmd_len=32768 fi ;; *) lt_cv_sys_max_cmd_len=`(getconf ARG_MAX) 2> /dev/null` if test -n "$lt_cv_sys_max_cmd_len" && \ test undefined != "$lt_cv_sys_max_cmd_len"; then lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \/ 4` lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \* 3` else # Make teststring a little bigger before we do anything with it. # a 1K string should be a reasonable start. for i in 1 2 3 4 5 6 7 8; do teststring=$teststring$teststring done SHELL=${SHELL-${CONFIG_SHELL-/bin/sh}} # If test is not a shell built-in, we'll probably end up computing a # maximum length that is only half of the actual maximum length, but # we can't tell. while { test X`env echo "$teststring$teststring" 2>/dev/null` \ = "X$teststring$teststring"; } >/dev/null 2>&1 && test 17 != "$i" # 1/2 MB should be enough do i=`expr $i + 1` teststring=$teststring$teststring done # Only check the string length outside the loop. lt_cv_sys_max_cmd_len=`expr "X$teststring" : ".*" 2>&1` teststring= # Add a significant safety factor because C++ compilers can tack on # massive amounts of additional arguments before passing them to the # linker. It appears as though 1/2 is a usable value. lt_cv_sys_max_cmd_len=`expr $lt_cv_sys_max_cmd_len \/ 2` fi ;; esac ]) if test -n "$lt_cv_sys_max_cmd_len"; then AC_MSG_RESULT($lt_cv_sys_max_cmd_len) else AC_MSG_RESULT(none) fi max_cmd_len=$lt_cv_sys_max_cmd_len _LT_DECL([], [max_cmd_len], [0], [What is the maximum length of a command?]) ])# LT_CMD_MAX_LEN # Old name: AU_ALIAS([AC_LIBTOOL_SYS_MAX_CMD_LEN], [LT_CMD_MAX_LEN]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_SYS_MAX_CMD_LEN], []) # _LT_HEADER_DLFCN # ---------------- m4_defun([_LT_HEADER_DLFCN], [AC_CHECK_HEADERS([dlfcn.h], [], [], [AC_INCLUDES_DEFAULT])dnl ])# _LT_HEADER_DLFCN # _LT_TRY_DLOPEN_SELF (ACTION-IF-TRUE, ACTION-IF-TRUE-W-USCORE, # ACTION-IF-FALSE, ACTION-IF-CROSS-COMPILING) # ---------------------------------------------------------------- m4_defun([_LT_TRY_DLOPEN_SELF], [m4_require([_LT_HEADER_DLFCN])dnl if test yes = "$cross_compiling"; then : [$4] else lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2 lt_status=$lt_dlunknown cat > conftest.$ac_ext <<_LT_EOF [#line $LINENO "configure" #include "confdefs.h" #if HAVE_DLFCN_H #include #endif #include #ifdef RTLD_GLOBAL # define LT_DLGLOBAL RTLD_GLOBAL #else # ifdef DL_GLOBAL # define LT_DLGLOBAL DL_GLOBAL # else # define LT_DLGLOBAL 0 # endif #endif /* We may have to define LT_DLLAZY_OR_NOW in the command line if we find out it does not work in some platform. */ #ifndef LT_DLLAZY_OR_NOW # ifdef RTLD_LAZY # define LT_DLLAZY_OR_NOW RTLD_LAZY # else # ifdef DL_LAZY # define LT_DLLAZY_OR_NOW DL_LAZY # else # ifdef RTLD_NOW # define LT_DLLAZY_OR_NOW RTLD_NOW # else # ifdef DL_NOW # define LT_DLLAZY_OR_NOW DL_NOW # else # define LT_DLLAZY_OR_NOW 0 # endif # endif # endif # endif #endif /* When -fvisibility=hidden is used, assume the code has been annotated correspondingly for the symbols needed. */ #if defined __GNUC__ && (((__GNUC__ == 3) && (__GNUC_MINOR__ >= 3)) || (__GNUC__ > 3)) int fnord () __attribute__((visibility("default"))); #endif int fnord () { return 42; } int main () { void *self = dlopen (0, LT_DLGLOBAL|LT_DLLAZY_OR_NOW); int status = $lt_dlunknown; if (self) { if (dlsym (self,"fnord")) status = $lt_dlno_uscore; else { if (dlsym( self,"_fnord")) status = $lt_dlneed_uscore; else puts (dlerror ()); } /* dlclose (self); */ } else puts (dlerror ()); return status; }] _LT_EOF if AC_TRY_EVAL(ac_link) && test -s "conftest$ac_exeext" 2>/dev/null; then (./conftest; exit; ) >&AS_MESSAGE_LOG_FD 2>/dev/null lt_status=$? case x$lt_status in x$lt_dlno_uscore) $1 ;; x$lt_dlneed_uscore) $2 ;; x$lt_dlunknown|x*) $3 ;; esac else : # compilation failed $3 fi fi rm -fr conftest* ])# _LT_TRY_DLOPEN_SELF # LT_SYS_DLOPEN_SELF # ------------------ AC_DEFUN([LT_SYS_DLOPEN_SELF], [m4_require([_LT_HEADER_DLFCN])dnl if test yes != "$enable_dlopen"; then enable_dlopen=unknown enable_dlopen_self=unknown enable_dlopen_self_static=unknown else lt_cv_dlopen=no lt_cv_dlopen_libs= case $host_os in beos*) lt_cv_dlopen=load_add_on lt_cv_dlopen_libs= lt_cv_dlopen_self=yes ;; mingw* | pw32* | cegcc*) lt_cv_dlopen=LoadLibrary lt_cv_dlopen_libs= ;; cygwin*) lt_cv_dlopen=dlopen lt_cv_dlopen_libs= ;; darwin*) # if libdl is installed we need to link against it AC_CHECK_LIB([dl], [dlopen], [lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-ldl],[ lt_cv_dlopen=dyld lt_cv_dlopen_libs= lt_cv_dlopen_self=yes ]) ;; tpf*) # Don't try to run any link tests for TPF. We know it's impossible # because TPF is a cross-compiler, and we know how we open DSOs. lt_cv_dlopen=dlopen lt_cv_dlopen_libs= lt_cv_dlopen_self=no ;; *) AC_CHECK_FUNC([shl_load], [lt_cv_dlopen=shl_load], [AC_CHECK_LIB([dld], [shl_load], [lt_cv_dlopen=shl_load lt_cv_dlopen_libs=-ldld], [AC_CHECK_FUNC([dlopen], [lt_cv_dlopen=dlopen], [AC_CHECK_LIB([dl], [dlopen], [lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-ldl], [AC_CHECK_LIB([svld], [dlopen], [lt_cv_dlopen=dlopen lt_cv_dlopen_libs=-lsvld], [AC_CHECK_LIB([dld], [dld_link], [lt_cv_dlopen=dld_link lt_cv_dlopen_libs=-ldld]) ]) ]) ]) ]) ]) ;; esac if test no = "$lt_cv_dlopen"; then enable_dlopen=no else enable_dlopen=yes fi case $lt_cv_dlopen in dlopen) save_CPPFLAGS=$CPPFLAGS test yes = "$ac_cv_header_dlfcn_h" && CPPFLAGS="$CPPFLAGS -DHAVE_DLFCN_H" save_LDFLAGS=$LDFLAGS wl=$lt_prog_compiler_wl eval LDFLAGS=\"\$LDFLAGS $export_dynamic_flag_spec\" save_LIBS=$LIBS LIBS="$lt_cv_dlopen_libs $LIBS" AC_CACHE_CHECK([whether a program can dlopen itself], lt_cv_dlopen_self, [dnl _LT_TRY_DLOPEN_SELF( lt_cv_dlopen_self=yes, lt_cv_dlopen_self=yes, lt_cv_dlopen_self=no, lt_cv_dlopen_self=cross) ]) if test yes = "$lt_cv_dlopen_self"; then wl=$lt_prog_compiler_wl eval LDFLAGS=\"\$LDFLAGS $lt_prog_compiler_static\" AC_CACHE_CHECK([whether a statically linked program can dlopen itself], lt_cv_dlopen_self_static, [dnl _LT_TRY_DLOPEN_SELF( lt_cv_dlopen_self_static=yes, lt_cv_dlopen_self_static=yes, lt_cv_dlopen_self_static=no, lt_cv_dlopen_self_static=cross) ]) fi CPPFLAGS=$save_CPPFLAGS LDFLAGS=$save_LDFLAGS LIBS=$save_LIBS ;; esac case $lt_cv_dlopen_self in yes|no) enable_dlopen_self=$lt_cv_dlopen_self ;; *) enable_dlopen_self=unknown ;; esac case $lt_cv_dlopen_self_static in yes|no) enable_dlopen_self_static=$lt_cv_dlopen_self_static ;; *) enable_dlopen_self_static=unknown ;; esac fi _LT_DECL([dlopen_support], [enable_dlopen], [0], [Whether dlopen is supported]) _LT_DECL([dlopen_self], [enable_dlopen_self], [0], [Whether dlopen of programs is supported]) _LT_DECL([dlopen_self_static], [enable_dlopen_self_static], [0], [Whether dlopen of statically linked programs is supported]) ])# LT_SYS_DLOPEN_SELF # Old name: AU_ALIAS([AC_LIBTOOL_DLOPEN_SELF], [LT_SYS_DLOPEN_SELF]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_LIBTOOL_DLOPEN_SELF], []) # _LT_COMPILER_C_O([TAGNAME]) # --------------------------- # Check to see if options -c and -o are simultaneously supported by compiler. # This macro does not hard code the compiler like AC_PROG_CC_C_O. m4_defun([_LT_COMPILER_C_O], [m4_require([_LT_DECL_SED])dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl m4_require([_LT_TAG_COMPILER])dnl AC_CACHE_CHECK([if $compiler supports -c -o file.$ac_objext], [_LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)], [_LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)=no $RM -r conftest 2>/dev/null mkdir conftest cd conftest mkdir out echo "$lt_simple_compile_test_code" > conftest.$ac_ext lt_compiler_flag="-o out/conftest2.$ac_objext" # Insert the option either (1) after the last *FLAGS variable, or # (2) before a word containing "conftest.", or (3) at the end. # Note that $ac_compile itself does not contain backslashes and begins # with a dollar sign (not a hyphen), so the echo should work correctly. lt_compile=`echo "$ac_compile" | $SED \ -e 's:.*FLAGS}\{0,1\} :&$lt_compiler_flag :; t' \ -e 's: [[^ ]]*conftest\.: $lt_compiler_flag&:; t' \ -e 's:$: $lt_compiler_flag:'` (eval echo "\"\$as_me:$LINENO: $lt_compile\"" >&AS_MESSAGE_LOG_FD) (eval "$lt_compile" 2>out/conftest.err) ac_status=$? cat out/conftest.err >&AS_MESSAGE_LOG_FD echo "$as_me:$LINENO: \$? = $ac_status" >&AS_MESSAGE_LOG_FD if (exit $ac_status) && test -s out/conftest2.$ac_objext then # The compiler can only warn and ignore the option if not recognized # So say no if there are warnings $ECHO "$_lt_compiler_boilerplate" | $SED '/^$/d' > out/conftest.exp $SED '/^$/d; /^ *+/d' out/conftest.err >out/conftest.er2 if test ! -s out/conftest.er2 || diff out/conftest.exp out/conftest.er2 >/dev/null; then _LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)=yes fi fi chmod u+w . 2>&AS_MESSAGE_LOG_FD $RM conftest* # SGI C++ compiler will create directory out/ii_files/ for # template instantiation test -d out/ii_files && $RM out/ii_files/* && rmdir out/ii_files $RM out/* && rmdir out cd .. $RM -r conftest $RM conftest* ]) _LT_TAGDECL([compiler_c_o], [lt_cv_prog_compiler_c_o], [1], [Does compiler simultaneously support -c and -o options?]) ])# _LT_COMPILER_C_O # _LT_COMPILER_FILE_LOCKS([TAGNAME]) # ---------------------------------- # Check to see if we can do hard links to lock some files if needed m4_defun([_LT_COMPILER_FILE_LOCKS], [m4_require([_LT_ENABLE_LOCK])dnl m4_require([_LT_FILEUTILS_DEFAULTS])dnl _LT_COMPILER_C_O([$1]) hard_links=nottested if test no = "$_LT_TAGVAR(lt_cv_prog_compiler_c_o, $1)" && test no != "$need_locks"; then # do not overwrite the value of need_locks provided by the user AC_MSG_CHECKING([if we can lock with hard links]) hard_links=yes $RM conftest* ln conftest.a conftest.b 2>/dev/null && hard_links=no touch conftest.a ln conftest.a conftest.b 2>&5 || hard_links=no ln conftest.a conftest.b 2>/dev/null && hard_links=no AC_MSG_RESULT([$hard_links]) if test no = "$hard_links"; then AC_MSG_WARN(['$CC' does not support '-c -o', so 'make -j' may be unsafe]) need_locks=warn fi else need_locks=no fi _LT_DECL([], [need_locks], [1], [Must we lock files when doing compilation?]) ])# _LT_COMPILER_FILE_LOCKS # _LT_CHECK_OBJDIR # ---------------- m4_defun([_LT_CHECK_OBJDIR], [AC_CACHE_CHECK([for objdir], [lt_cv_objdir], [rm -f .libs 2>/dev/null mkdir .libs 2>/dev/null if test -d .libs; then lt_cv_objdir=.libs else # MS-DOS does not allow filenames that begin with a dot. lt_cv_objdir=_libs fi rmdir .libs 2>/dev/null]) objdir=$lt_cv_objdir _LT_DECL([], [objdir], [0], [The name of the directory that contains temporary libtool files])dnl m4_pattern_allow([LT_OBJDIR])dnl AC_DEFINE_UNQUOTED([LT_OBJDIR], "$lt_cv_objdir/", [Define to the sub-directory where libtool stores uninstalled libraries.]) ])# _LT_CHECK_OBJDIR # _LT_LINKER_HARDCODE_LIBPATH([TAGNAME]) # -------------------------------------- # Check hardcoding attributes. m4_defun([_LT_LINKER_HARDCODE_LIBPATH], [AC_MSG_CHECKING([how to hardcode library paths into programs]) _LT_TAGVAR(hardcode_action, $1)= if test -n "$_LT_TAGVAR(hardcode_libdir_flag_spec, $1)" || test -n "$_LT_TAGVAR(runpath_var, $1)" || test yes = "$_LT_TAGVAR(hardcode_automatic, $1)"; then # We can hardcode non-existent directories. if test no != "$_LT_TAGVAR(hardcode_direct, $1)" && # If the only mechanism to avoid hardcoding is shlibpath_var, we # have to relink, otherwise we might link with an installed library # when we should be linking with a yet-to-be-installed one ## test no != "$_LT_TAGVAR(hardcode_shlibpath_var, $1)" && test no != "$_LT_TAGVAR(hardcode_minus_L, $1)"; then # Linking always hardcodes the temporary library directory. _LT_TAGVAR(hardcode_action, $1)=relink else # We can link without hardcoding, and we can hardcode nonexisting dirs. _LT_TAGVAR(hardcode_action, $1)=immediate fi else # We cannot hardcode anything, or else we can only hardcode existing # directories. _LT_TAGVAR(hardcode_action, $1)=unsupported fi AC_MSG_RESULT([$_LT_TAGVAR(hardcode_action, $1)]) if test relink = "$_LT_TAGVAR(hardcode_action, $1)" || test yes = "$_LT_TAGVAR(inherit_rpath, $1)"; then # Fast installation is not supported enable_fast_install=no elif test yes = "$shlibpath_overrides_runpath" || test no = "$enable_shared"; 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*) case $LD in # libtool.m4 will add one of these switches to LD *-32|*"-32 "|*-melf32bsmip|*"-melf32bsmip ") libsuff= shlibsuff= libmagic=32-bit;; *-n32|*"-n32 "|*-melf32bmipn32|*"-melf32bmipn32 ") libsuff=32 shlibsuff=N32 libmagic=N32;; *-64|*"-64 "|*-melf64bmip|*"-melf64bmip ") libsuff=64 shlibsuff=64 libmagic=64-bit;; *) libsuff= shlibsuff= libmagic=never-match;; esac ;; esac shlibpath_var=LD_LIBRARY${shlibsuff}_PATH shlibpath_overrides_runpath=no sys_lib_search_path_spec="/usr/lib$libsuff /lib$libsuff /usr/local/lib$libsuff" sys_lib_dlsearch_path_spec="/usr/lib$libsuff /lib$libsuff" hardcode_into_libs=yes ;; # No shared lib support for Linux oldld, aout, or coff. linux*oldld* | linux*aout* | linux*coff*) dynamic_linker=no ;; linux*android*) version_type=none # Android doesn't support versioned libraries. need_lib_prefix=no need_version=no library_names_spec='$libname$release$shared_ext' soname_spec='$libname$release$shared_ext' finish_cmds= shlibpath_var=LD_LIBRARY_PATH shlibpath_overrides_runpath=yes # This implies no fast_install, which is unacceptable. # Some rework will be needed to allow for fast_install # before this can be enabled. hardcode_into_libs=yes dynamic_linker='Android linker' # Don't embed -rpath directories since the linker doesn't support them. _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-L$libdir' ;; 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sni) lt_cv_file_magic_cmd='/bin/file' lt_cv_deplibs_check_method="file_magic ELF [[0-9]][[0-9]]*-bit [[LM]]SB dynamic lib" lt_cv_file_magic_test_file=/lib/libc.so ;; siemens) lt_cv_deplibs_check_method=pass_all ;; pc) lt_cv_deplibs_check_method=pass_all ;; esac ;; tpf*) lt_cv_deplibs_check_method=pass_all ;; os2*) lt_cv_deplibs_check_method=pass_all ;; esac ]) file_magic_glob= want_nocaseglob=no if test "$build" = "$host"; then case $host_os in mingw* | pw32*) if ( shopt | grep nocaseglob ) >/dev/null 2>&1; then want_nocaseglob=yes else file_magic_glob=`echo aAbBcCdDeEfFgGhHiIjJkKlLmMnNoOpPqQrRsStTuUvVwWxXyYzZ | $SED -e "s/\(..\)/s\/[[\1]]\/[[\1]]\/g;/g"` fi ;; esac fi file_magic_cmd=$lt_cv_file_magic_cmd deplibs_check_method=$lt_cv_deplibs_check_method test -z "$deplibs_check_method" && deplibs_check_method=unknown _LT_DECL([], [deplibs_check_method], [1], [Method to check whether dependent libraries are shared objects]) _LT_DECL([], [file_magic_cmd], [1], [Command to use when deplibs_check_method = "file_magic"]) _LT_DECL([], [file_magic_glob], [1], [How to find potential files when deplibs_check_method = "file_magic"]) _LT_DECL([], [want_nocaseglob], [1], [Find potential files using nocaseglob when deplibs_check_method = "file_magic"]) ])# _LT_CHECK_MAGIC_METHOD # LT_PATH_NM # ---------- # find the pathname to a BSD- or MS-compatible name lister AC_DEFUN([LT_PATH_NM], [AC_REQUIRE([AC_PROG_CC])dnl AC_CACHE_CHECK([for BSD- or MS-compatible name lister (nm)], lt_cv_path_NM, [if test -n "$NM"; 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then MANIFEST_TOOL=: fi _LT_DECL([], [MANIFEST_TOOL], [1], [Manifest tool])dnl ])# _LT_PATH_MANIFEST_TOOL # _LT_DLL_DEF_P([FILE]) # --------------------- # True iff FILE is a Windows DLL '.def' file. # Keep in sync with func_dll_def_p in the libtool script AC_DEFUN([_LT_DLL_DEF_P], [dnl test DEF = "`$SED -n dnl -e '\''s/^[[ ]]*//'\'' dnl Strip leading whitespace -e '\''/^\(;.*\)*$/d'\'' dnl Delete empty lines and comments -e '\''s/^\(EXPORTS\|LIBRARY\)\([[ ]].*\)*$/DEF/p'\'' dnl -e q dnl Only consider the first "real" line $1`" dnl ])# _LT_DLL_DEF_P # LT_LIB_M # -------- # check for math library AC_DEFUN([LT_LIB_M], [AC_REQUIRE([AC_CANONICAL_HOST])dnl LIBM= case $host in *-*-beos* | *-*-cegcc* | *-*-cygwin* | *-*-haiku* | *-*-pw32* | *-*-darwin*) # These system don't have libm, or don't need it ;; *-ncr-sysv4.3*) AC_CHECK_LIB(mw, _mwvalidcheckl, LIBM=-lmw) AC_CHECK_LIB(m, cos, LIBM="$LIBM -lm") ;; *) AC_CHECK_LIB(m, cos, LIBM=-lm) ;; esac AC_SUBST([LIBM]) ])# LT_LIB_M # Old name: AU_ALIAS([AC_CHECK_LIBM], [LT_LIB_M]) dnl aclocal-1.4 backwards compatibility: dnl AC_DEFUN([AC_CHECK_LIBM], []) # _LT_COMPILER_NO_RTTI([TAGNAME]) # ------------------------------- m4_defun([_LT_COMPILER_NO_RTTI], [m4_require([_LT_TAG_COMPILER])dnl _LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)= if test yes = "$GCC"; 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What could be older than Ultrix?!! ;)] # Character class describing NM global symbol codes. symcode='[[BCDEGRST]]' # Regexp to match symbols that can be accessed directly from C. sympat='\([[_A-Za-z]][[_A-Za-z0-9]]*\)' # Define system-specific variables. case $host_os in aix*) symcode='[[BCDT]]' ;; cygwin* | mingw* | pw32* | cegcc*) symcode='[[ABCDGISTW]]' ;; hpux*) if test ia64 = "$host_cpu"; then symcode='[[ABCDEGRST]]' fi ;; irix* | nonstopux*) symcode='[[BCDEGRST]]' ;; osf*) symcode='[[BCDEGQRST]]' ;; solaris*) symcode='[[BDRT]]' ;; sco3.2v5*) symcode='[[DT]]' ;; sysv4.2uw2*) symcode='[[DT]]' ;; sysv5* | sco5v6* | unixware* | OpenUNIX*) symcode='[[ABDT]]' ;; sysv4) symcode='[[DFNSTU]]' ;; esac # If we're using GNU nm, then use its standard symbol codes. case `$NM -V 2>&1` in *GNU* | *'with BFD'*) symcode='[[ABCDGIRSTW]]' ;; esac if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Gets list of data symbols to import. lt_cv_sys_global_symbol_to_import="sed -n -e 's/^I .* \(.*\)$/\1/p'" # Adjust the below global symbol transforms to fixup imported variables. lt_cdecl_hook=" -e 's/^I .* \(.*\)$/extern __declspec(dllimport) char \1;/p'" lt_c_name_hook=" -e 's/^I .* \(.*\)$/ {\"\1\", (void *) 0},/p'" lt_c_name_lib_hook="\ -e 's/^I .* \(lib.*\)$/ {\"\1\", (void *) 0},/p'\ -e 's/^I .* \(.*\)$/ {\"lib\1\", (void *) 0},/p'" else # Disable hooks by default. lt_cv_sys_global_symbol_to_import= lt_cdecl_hook= lt_c_name_hook= lt_c_name_lib_hook= fi # Transform an extracted symbol line into a proper C declaration. # Some systems (esp. on ia64) link data and code symbols differently, # so use this general approach. lt_cv_sys_global_symbol_to_cdecl="sed -n"\ $lt_cdecl_hook\ " -e 's/^T .* \(.*\)$/extern int \1();/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/extern char \1;/p'" # Transform an extracted symbol line into symbol name and symbol address lt_cv_sys_global_symbol_to_c_name_address="sed -n"\ $lt_c_name_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/p'" # Transform an extracted symbol line into symbol name with lib prefix and # symbol address. lt_cv_sys_global_symbol_to_c_name_address_lib_prefix="sed -n"\ $lt_c_name_lib_hook\ " -e 's/^: \(.*\) .*$/ {\"\1\", (void *) 0},/p'"\ " -e 's/^$symcode$symcode* .* \(lib.*\)$/ {\"\1\", (void *) \&\1},/p'"\ " -e 's/^$symcode$symcode* .* \(.*\)$/ {\"lib\1\", (void *) \&\1},/p'" # Handle CRLF in mingw tool chain opt_cr= case $build_os in mingw*) opt_cr=`$ECHO 'x\{0,1\}' | tr x '\015'` # option cr in regexp ;; esac # Try without a prefix underscore, then with it. for ac_symprfx in "" "_"; do # Transform symcode, sympat, and symprfx into a raw symbol and a C symbol. symxfrm="\\1 $ac_symprfx\\2 \\2" # Write the raw and C identifiers. if test "$lt_cv_nm_interface" = "MS dumpbin"; then # Fake it for dumpbin and say T for any non-static function, # D for any global variable and I for any imported variable. # Also find C++ and __fastcall symbols from MSVC++, # which start with @ or ?. lt_cv_sys_global_symbol_pipe="$AWK ['"\ " {last_section=section; section=\$ 3};"\ " /^COFF SYMBOL TABLE/{for(i in hide) delete hide[i]};"\ " /Section length .*#relocs.*(pick any)/{hide[last_section]=1};"\ " /^ *Symbol name *: /{split(\$ 0,sn,\":\"); si=substr(sn[2],2)};"\ " /^ *Type *: code/{print \"T\",si,substr(si,length(prfx))};"\ " /^ *Type *: data/{print \"I\",si,substr(si,length(prfx))};"\ " \$ 0!~/External *\|/{next};"\ " / 0+ UNDEF /{next}; / UNDEF \([^|]\)*()/{next};"\ " {if(hide[section]) next};"\ " {f=\"D\"}; \$ 0~/\(\).*\|/{f=\"T\"};"\ " {split(\$ 0,a,/\||\r/); split(a[2],s)};"\ " s[1]~/^[@?]/{print f,s[1],s[1]; next};"\ " s[1]~prfx {split(s[1],t,\"@\"); print f,t[1],substr(t[1],length(prfx))}"\ " ' prfx=^$ac_symprfx]" else lt_cv_sys_global_symbol_pipe="sed -n -e 's/^.*[[ ]]\($symcode$symcode*\)[[ ]][[ ]]*$ac_symprfx$sympat$opt_cr$/$symxfrm/p'" fi lt_cv_sys_global_symbol_pipe="$lt_cv_sys_global_symbol_pipe | sed '/ __gnu_lto/d'" # Check to see that the pipe works correctly. pipe_works=no rm -f conftest* cat > conftest.$ac_ext <<_LT_EOF #ifdef __cplusplus extern "C" { #endif char nm_test_var; void nm_test_func(void); void nm_test_func(void){} #ifdef __cplusplus } #endif int main(){nm_test_var='a';nm_test_func();return(0);} _LT_EOF if AC_TRY_EVAL(ac_compile); then # Now try to grab the symbols. nlist=conftest.nm if AC_TRY_EVAL(NM conftest.$ac_objext \| "$lt_cv_sys_global_symbol_pipe" \> $nlist) && test -s "$nlist"; then # Try sorting and uniquifying the output. if sort "$nlist" | uniq > "$nlist"T; then mv -f "$nlist"T "$nlist" else rm -f "$nlist"T fi # Make sure that we snagged all the symbols we need. if $GREP ' nm_test_var$' "$nlist" >/dev/null; then if $GREP ' nm_test_func$' "$nlist" >/dev/null; then cat <<_LT_EOF > conftest.$ac_ext /* Keep this code in sync between libtool.m4, ltmain, lt_system.h, and tests. */ #if defined _WIN32 || defined __CYGWIN__ || defined _WIN32_WCE /* DATA imports from DLLs on WIN32 can't be const, because runtime relocations are performed -- see ld's documentation on pseudo-relocs. */ # define LT@&t@_DLSYM_CONST #elif defined __osf__ /* This system does not cope well with relocations in const data. */ # define LT@&t@_DLSYM_CONST #else # define LT@&t@_DLSYM_CONST const #endif #ifdef __cplusplus extern "C" { #endif _LT_EOF # Now generate the symbol file. eval "$lt_cv_sys_global_symbol_to_cdecl"' < "$nlist" | $GREP -v main >> conftest.$ac_ext' cat <<_LT_EOF >> conftest.$ac_ext /* The mapping between symbol names and symbols. */ LT@&t@_DLSYM_CONST struct { const char *name; void *address; } lt__PROGRAM__LTX_preloaded_symbols[[]] = { { "@PROGRAM@", (void *) 0 }, _LT_EOF $SED "s/^$symcode$symcode* .* \(.*\)$/ {\"\1\", (void *) \&\1},/" < "$nlist" | $GREP -v main >> conftest.$ac_ext cat <<\_LT_EOF >> conftest.$ac_ext {0, (void *) 0} }; /* This works around a problem in FreeBSD linker */ #ifdef FREEBSD_WORKAROUND static const void *lt_preloaded_setup() { return lt__PROGRAM__LTX_preloaded_symbols; } #endif #ifdef __cplusplus } #endif _LT_EOF # Now try linking the two files. mv conftest.$ac_objext conftstm.$ac_objext lt_globsym_save_LIBS=$LIBS lt_globsym_save_CFLAGS=$CFLAGS LIBS=conftstm.$ac_objext CFLAGS="$CFLAGS$_LT_TAGVAR(lt_prog_compiler_no_builtin_flag, $1)" if AC_TRY_EVAL(ac_link) && test -s conftest$ac_exeext; then pipe_works=yes fi LIBS=$lt_globsym_save_LIBS CFLAGS=$lt_globsym_save_CFLAGS else echo "cannot find nm_test_func in $nlist" >&AS_MESSAGE_LOG_FD fi else echo "cannot find nm_test_var in $nlist" >&AS_MESSAGE_LOG_FD fi else echo "cannot run $lt_cv_sys_global_symbol_pipe" >&AS_MESSAGE_LOG_FD fi else echo "$progname: failed program was:" >&AS_MESSAGE_LOG_FD cat conftest.$ac_ext >&5 fi rm -rf conftest* conftst* # Do not use the global_symbol_pipe unless it works. if test yes = "$pipe_works"; then break else lt_cv_sys_global_symbol_pipe= fi done ]) if test -z "$lt_cv_sys_global_symbol_pipe"; then lt_cv_sys_global_symbol_to_cdecl= fi if test -z "$lt_cv_sys_global_symbol_pipe$lt_cv_sys_global_symbol_to_cdecl"; then AC_MSG_RESULT(failed) else AC_MSG_RESULT(ok) fi # Response file support. if test "$lt_cv_nm_interface" = "MS dumpbin"; then nm_file_list_spec='@' elif $NM --help 2>/dev/null | grep '[[@]]FILE' >/dev/null; then nm_file_list_spec='@' fi _LT_DECL([global_symbol_pipe], [lt_cv_sys_global_symbol_pipe], [1], [Take the output of nm and produce a listing of raw symbols and C names]) _LT_DECL([global_symbol_to_cdecl], [lt_cv_sys_global_symbol_to_cdecl], [1], [Transform the output of nm in a proper C declaration]) _LT_DECL([global_symbol_to_import], [lt_cv_sys_global_symbol_to_import], [1], [Transform the output of nm into a list of symbols to manually relocate]) _LT_DECL([global_symbol_to_c_name_address], [lt_cv_sys_global_symbol_to_c_name_address], [1], [Transform the output of nm in a C name address pair]) _LT_DECL([global_symbol_to_c_name_address_lib_prefix], [lt_cv_sys_global_symbol_to_c_name_address_lib_prefix], [1], [Transform the output of nm in a C name address pair when lib prefix is needed]) _LT_DECL([nm_interface], [lt_cv_nm_interface], [1], [The name lister interface]) _LT_DECL([], [nm_file_list_spec], [1], [Specify filename containing input files for $NM]) ]) # _LT_CMD_GLOBAL_SYMBOLS # _LT_COMPILER_PIC([TAGNAME]) # --------------------------- m4_defun([_LT_COMPILER_PIC], [m4_require([_LT_TAG_COMPILER])dnl _LT_TAGVAR(lt_prog_compiler_wl, $1)= _LT_TAGVAR(lt_prog_compiler_pic, $1)= _LT_TAGVAR(lt_prog_compiler_static, $1)= m4_if([$1], [CXX], [ # C++ specific cases for pic, static, wl, etc. if test yes = "$GXX"; then _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' case $host_os in aix*) # All AIX code is PIC. if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' fi _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; m68k) # FIXME: we need at least 68020 code to build shared libraries, but # adding the '-m68020' flag to GCC prevents building anything better, # like '-m68040'. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-m68020 -resident32 -malways-restore-a4' ;; esac ;; beos* | irix5* | irix6* | nonstopux* | osf3* | osf4* | osf5*) # PIC is the default for these OSes. ;; mingw* | cygwin* | os2* | pw32* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). # Although the cygwin gcc ignores -fPIC, still need this for old-style # (--disable-auto-import) libraries m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) case $host_os in os2*) _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-static' ;; esac ;; darwin* | rhapsody*) # PIC is the default on this platform # Common symbols not allowed in MH_DYLIB files _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fno-common' ;; *djgpp*) # DJGPP does not support shared libraries at all _LT_TAGVAR(lt_prog_compiler_pic, $1)= ;; haiku*) # PIC is the default for Haiku. # The "-static" flag exists, but is broken. _LT_TAGVAR(lt_prog_compiler_static, $1)= ;; interix[[3-9]]*) # Interix 3.x gcc -fpic/-fPIC options generate broken code. # Instead, we relocate shared libraries at runtime. ;; sysv4*MP*) if test -d /usr/nec; then _LT_TAGVAR(lt_prog_compiler_pic, $1)=-Kconform_pic fi ;; hpux*) # PIC is the default for 64-bit PA HP-UX, but not for 32-bit # PA HP-UX. On IA64 HP-UX, PIC is the default but the pic flag # sets the default TLS model and affects inlining. case $host_cpu in hppa*64*) ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac ;; *qnx* | *nto*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac else case $host_os in aix[[4-9]]*) # All AIX code is PIC. if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' else _LT_TAGVAR(lt_prog_compiler_static, $1)='-bnso -bI:/lib/syscalls.exp' fi ;; chorus*) case $cc_basename in cxch68*) # Green Hills C++ Compiler # _LT_TAGVAR(lt_prog_compiler_static, $1)="--no_auto_instantiation -u __main -u __premain -u _abort -r $COOL_DIR/lib/libOrb.a $MVME_DIR/lib/CC/libC.a $MVME_DIR/lib/classix/libcx.s.a" ;; esac ;; mingw* | cygwin* | os2* | pw32* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) ;; dgux*) case $cc_basename in ec++*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' ;; ghcx*) # Green Hills C++ Compiler _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' ;; *) ;; esac ;; freebsd* | dragonfly*) # FreeBSD uses GNU C++ ;; hpux9* | hpux10* | hpux11*) case $cc_basename in CC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-a ${wl}archive' if test ia64 != "$host_cpu"; then _LT_TAGVAR(lt_prog_compiler_pic, $1)='+Z' fi ;; aCC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-a ${wl}archive' case $host_cpu in hppa*64*|ia64*) # +Z the default ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='+Z' ;; esac ;; *) ;; esac ;; interix*) # This is c89, which is MS Visual C++ (no shared libs) # Anyone wants to do a port? ;; irix5* | irix6* | nonstopux*) case $cc_basename in CC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' # CC pic flag -KPIC is the default. ;; *) ;; esac ;; linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) case $cc_basename in KCC*) # KAI C++ Compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='--backend -Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; ecpc* ) # old Intel C++ for x86_64, which still supported -KPIC. _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; icpc* ) # Intel C++, used to be incompatible with GCC. # ICC 10 doesn't accept -KPIC any more. _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; pgCC* | pgcpp*) # Portland Group C++ compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; cxx*) # Compaq C++ # Make sure the PIC flag is empty. It appears that all Alpha # Linux and Compaq Tru64 Unix objects are PIC. _LT_TAGVAR(lt_prog_compiler_pic, $1)= _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; xlc* | xlC* | bgxl[[cC]]* | mpixl[[cC]]*) # IBM XL 8.0, 9.0 on PPC and BlueGene _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-qpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-qstaticlink' ;; *) case `$CC -V 2>&1 | sed 5q` in *Sun\ C*) # Sun C++ 5.9 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' ;; esac ;; esac ;; lynxos*) ;; m88k*) ;; mvs*) case $cc_basename in cxx*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-W c,exportall' ;; *) ;; esac ;; netbsd*) ;; *qnx* | *nto*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; osf3* | osf4* | osf5*) case $cc_basename in KCC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='--backend -Wl,' ;; RCC*) # Rational C++ 2.4.1 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' ;; cxx*) # Digital/Compaq C++ _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # Make sure the PIC flag is empty. It appears that all Alpha # Linux and Compaq Tru64 Unix objects are PIC. _LT_TAGVAR(lt_prog_compiler_pic, $1)= _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; *) ;; esac ;; psos*) ;; solaris*) case $cc_basename in CC* | sunCC*) # Sun C++ 4.2, 5.x and Centerline C++ _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' ;; gcx*) # Green Hills C++ Compiler _LT_TAGVAR(lt_prog_compiler_pic, $1)='-PIC' ;; *) ;; esac ;; sunos4*) case $cc_basename in CC*) # Sun C++ 4.x _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; lcc*) # Lucid _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' ;; *) ;; esac ;; sysv5* | unixware* | sco3.2v5* | sco5v6* | OpenUNIX*) case $cc_basename in CC*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; esac ;; tandem*) case $cc_basename in NCC*) # NonStop-UX NCC 3.20 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' ;; *) ;; esac ;; vxworks*) ;; *) _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no ;; esac fi ], [ if test yes = "$GCC"; then _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' case $host_os in aix*) # All AIX code is PIC. if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' fi _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; amigaos*) case $host_cpu in powerpc) # see comment about AmigaOS4 .so support _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; m68k) # FIXME: we need at least 68020 code to build shared libraries, but # adding the '-m68020' flag to GCC prevents building anything better, # like '-m68040'. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-m68020 -resident32 -malways-restore-a4' ;; esac ;; beos* | irix5* | irix6* | nonstopux* | osf3* | osf4* | osf5*) # PIC is the default for these OSes. ;; mingw* | cygwin* | pw32* | os2* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). # Although the cygwin gcc ignores -fPIC, still need this for old-style # (--disable-auto-import) libraries m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) case $host_os in os2*) _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-static' ;; esac ;; darwin* | rhapsody*) # PIC is the default on this platform # Common symbols not allowed in MH_DYLIB files _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fno-common' ;; haiku*) # PIC is the default for Haiku. # The "-static" flag exists, but is broken. _LT_TAGVAR(lt_prog_compiler_static, $1)= ;; hpux*) # PIC is the default for 64-bit PA HP-UX, but not for 32-bit # PA HP-UX. On IA64 HP-UX, PIC is the default but the pic flag # sets the default TLS model and affects inlining. case $host_cpu in hppa*64*) # +Z the default ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac ;; interix[[3-9]]*) # Interix 3.x gcc -fpic/-fPIC options generate broken code. # Instead, we relocate shared libraries at runtime. ;; msdosdjgpp*) # Just because we use GCC doesn't mean we suddenly get shared libraries # on systems that don't support them. _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no enable_shared=no ;; *nto* | *qnx*) # QNX uses GNU C++, but need to define -shared option too, otherwise # it will coredump. _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC -shared' ;; sysv4*MP*) if test -d /usr/nec; then _LT_TAGVAR(lt_prog_compiler_pic, $1)=-Kconform_pic fi ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' ;; esac case $cc_basename in nvcc*) # Cuda Compiler Driver 2.2 _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Xlinker ' if test -n "$_LT_TAGVAR(lt_prog_compiler_pic, $1)"; then _LT_TAGVAR(lt_prog_compiler_pic, $1)="-Xcompiler $_LT_TAGVAR(lt_prog_compiler_pic, $1)" fi ;; esac else # PORTME Check for flag to pass linker flags through the system compiler. case $host_os in aix*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' if test ia64 = "$host_cpu"; then # AIX 5 now supports IA64 processor _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' else _LT_TAGVAR(lt_prog_compiler_static, $1)='-bnso -bI:/lib/syscalls.exp' fi ;; darwin* | rhapsody*) # PIC is the default on this platform # Common symbols not allowed in MH_DYLIB files _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fno-common' case $cc_basename in nagfor*) # NAG Fortran compiler _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,-Wl,,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-PIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; esac ;; mingw* | cygwin* | pw32* | os2* | cegcc*) # This hack is so that the source file can tell whether it is being # built for inclusion in a dll (and should export symbols for example). m4_if([$1], [GCJ], [], [_LT_TAGVAR(lt_prog_compiler_pic, $1)='-DDLL_EXPORT']) case $host_os in os2*) _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-static' ;; esac ;; hpux9* | hpux10* | hpux11*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # PIC is the default for IA64 HP-UX and 64-bit HP-UX, but # not for PA HP-UX. case $host_cpu in hppa*64*|ia64*) # +Z the default ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)='+Z' ;; esac # Is there a better lt_prog_compiler_static that works with the bundled CC? _LT_TAGVAR(lt_prog_compiler_static, $1)='$wl-a ${wl}archive' ;; irix5* | irix6* | nonstopux*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' # PIC (with -KPIC) is the default. _LT_TAGVAR(lt_prog_compiler_static, $1)='-non_shared' ;; linux* | k*bsd*-gnu | kopensolaris*-gnu | gnu*) case $cc_basename in # old Intel for x86_64, which still supported -KPIC. ecc*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; # icc used to be incompatible with GCC. # ICC 10 doesn't accept -KPIC any more. icc* | ifort*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; 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*) case `$CC -V 2>&1 | sed 5q` in *Sun\ Ceres\ Fortran* | *Sun*Fortran*\ [[1-7]].* | *Sun*Fortran*\ 8.[[0-3]]*) # Sun Fortran 8.3 passes all unrecognized flags to the linker _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='' ;; *Sun\ F* | *Sun*Fortran*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Qoption ld ' ;; *Sun\ C*) # Sun C 5.9 _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' ;; *Intel*\ [[CF]]*Compiler*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-static' ;; *Portland\ Group*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-fpic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; esac ;; esac ;; newsos6) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; 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then _LT_TAGVAR(lt_prog_compiler_pic, $1)='-Kconform_pic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' fi ;; sysv5* | unixware* | sco3.2v5* | sco5v6* | OpenUNIX*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_pic, $1)='-KPIC' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; unicos*) _LT_TAGVAR(lt_prog_compiler_wl, $1)='-Wl,' _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no ;; uts4*) _LT_TAGVAR(lt_prog_compiler_pic, $1)='-pic' _LT_TAGVAR(lt_prog_compiler_static, $1)='-Bstatic' ;; *) _LT_TAGVAR(lt_prog_compiler_can_build_shared, $1)=no ;; esac fi ]) case $host_os in # For platforms that do not support PIC, -DPIC is meaningless: *djgpp*) _LT_TAGVAR(lt_prog_compiler_pic, $1)= ;; *) _LT_TAGVAR(lt_prog_compiler_pic, $1)="$_LT_TAGVAR(lt_prog_compiler_pic, $1)@&t@m4_if([$1],[],[ -DPIC],[m4_if([$1],[CXX],[ -DPIC],[])])" ;; esac AC_CACHE_CHECK([for $compiler option to produce PIC], [_LT_TAGVAR(lt_cv_prog_compiler_pic, $1)], [_LT_TAGVAR(lt_cv_prog_compiler_pic, $1)=$_LT_TAGVAR(lt_prog_compiler_pic, $1)]) _LT_TAGVAR(lt_prog_compiler_pic, $1)=$_LT_TAGVAR(lt_cv_prog_compiler_pic, $1) # # Check to make sure the PIC flag actually works. # if test -n "$_LT_TAGVAR(lt_prog_compiler_pic, $1)"; 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Moving up from 0x10000000 also allows more sbrk(2) space. _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-h,$soname $wl--image-base,`expr ${RANDOM-$$} % 4096 / 2 \* 262144 + 1342177280` -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='sed "s|^|_|" $export_symbols >$output_objdir/$soname.expsym~$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-h,$soname $wl--retain-symbols-file,$output_objdir/$soname.expsym $wl--image-base,`expr ${RANDOM-$$} % 4096 / 2 \* 262144 + 1342177280` -o $lib' ;; gnu* | linux* | tpf* | k*bsd*-gnu | kopensolaris*-gnu) tmp_diet=no if test linux-dietlibc = "$host_os"; then case $cc_basename in diet\ *) tmp_diet=yes;; # linux-dietlibc with static linking (!diet-dyn) esac fi if $LD --help 2>&1 | $EGREP ': supported targets:.* elf' > /dev/null \ && test no = "$tmp_diet" then tmp_addflag=' $pic_flag' tmp_sharedflag='-shared' case $cc_basename,$host_cpu in pgcc*) # Portland Group C compiler _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' tmp_addflag=' $pic_flag' ;; pgf77* | pgf90* | pgf95* | pgfortran*) # Portland Group f77 and f90 compilers _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' tmp_addflag=' $pic_flag -Mnomain' ;; ecc*,ia64* | icc*,ia64*) # Intel C compiler on ia64 tmp_addflag=' -i_dynamic' ;; efc*,ia64* | ifort*,ia64*) # Intel Fortran compiler on ia64 tmp_addflag=' -i_dynamic -nofor_main' ;; ifc* | ifort*) # Intel Fortran compiler tmp_addflag=' -nofor_main' ;; lf95*) # Lahey Fortran 8.1 _LT_TAGVAR(whole_archive_flag_spec, $1)= tmp_sharedflag='--shared' ;; nagfor*) # NAGFOR 5.3 tmp_sharedflag='-Wl,-shared' ;; xl[[cC]]* | bgxl[[cC]]* | mpixl[[cC]]*) # IBM XL C 8.0 on PPC (deal with xlf below) tmp_sharedflag='-qmkshrobj' tmp_addflag= ;; nvcc*) # Cuda Compiler Driver 2.2 _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' _LT_TAGVAR(compiler_needs_object, $1)=yes ;; esac case `$CC -V 2>&1 | sed 5q` in *Sun\ C*) # Sun C 5.9 _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive`new_convenience=; for conv in $convenience\"\"; do test -z \"$conv\" || new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' _LT_TAGVAR(compiler_needs_object, $1)=yes tmp_sharedflag='-G' ;; *Sun\ F*) # Sun Fortran 8.3 tmp_sharedflag='-G' ;; esac _LT_TAGVAR(archive_cmds, $1)='$CC '"$tmp_sharedflag""$tmp_addflag"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' if test yes = "$supports_anon_versioning"; then _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $output_objdir/$libname.ver~ cat $export_symbols | sed -e "s/\(.*\)/\1;/" >> $output_objdir/$libname.ver~ echo "local: *; };" >> $output_objdir/$libname.ver~ $CC '"$tmp_sharedflag""$tmp_addflag"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-version-script $wl$output_objdir/$libname.ver -o $lib' fi case $cc_basename in tcc*) _LT_TAGVAR(export_dynamic_flag_spec, $1)='-rdynamic' ;; xlf* | bgf* | bgxlf* | mpixlf*) # IBM XL Fortran 10.1 on PPC cannot create shared libs itself _LT_TAGVAR(whole_archive_flag_spec, $1)='--whole-archive$convenience --no-whole-archive' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath $wl$libdir' _LT_TAGVAR(archive_cmds, $1)='$LD -shared $libobjs $deplibs $linker_flags -soname $soname -o $lib' if test yes = "$supports_anon_versioning"; then _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $output_objdir/$libname.ver~ cat $export_symbols | sed -e "s/\(.*\)/\1;/" >> $output_objdir/$libname.ver~ echo "local: *; };" >> $output_objdir/$libname.ver~ $LD -shared $libobjs $deplibs $linker_flags -soname $soname -version-script $output_objdir/$libname.ver -o $lib' fi ;; esac else _LT_TAGVAR(ld_shlibs, $1)=no fi ;; netbsd*) if echo __ELF__ | $CC -E - | $GREP __ELF__ >/dev/null; then _LT_TAGVAR(archive_cmds, $1)='$LD -Bshareable $libobjs $deplibs $linker_flags -o $lib' wlarc= else _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' fi ;; solaris*) if $LD -v 2>&1 | $GREP 'BFD 2\.8' > /dev/null; then _LT_TAGVAR(ld_shlibs, $1)=no cat <<_LT_EOF 1>&2 *** Warning: The releases 2.8.* of the GNU linker cannot reliably *** create shared libraries on Solaris systems. Therefore, libtool *** is disabling shared libraries support. We urge you to upgrade GNU *** binutils to release 2.9.1 or newer. Another option is to modify *** your PATH or compiler configuration so that the native linker is *** used, and then restart. _LT_EOF elif $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' else _LT_TAGVAR(ld_shlibs, $1)=no fi ;; sysv5* | sco3.2v5* | sco5v6* | unixware* | OpenUNIX*) case `$LD -v 2>&1` in *\ [[01]].* | *\ 2.[[0-9]].* | *\ 2.1[[0-5]].*) _LT_TAGVAR(ld_shlibs, $1)=no cat <<_LT_EOF 1>&2 *** Warning: Releases of the GNU linker prior to 2.16.91.0.3 cannot *** reliably create shared libraries on SCO systems. Therefore, libtool *** is disabling shared libraries support. We urge you to upgrade GNU *** binutils to release 2.16.91.0.3 or newer. Another option is to modify *** your PATH or compiler configuration so that the native linker is *** used, and then restart. _LT_EOF ;; *) # For security reasons, it is highly recommended that you always # use absolute paths for naming shared libraries, and exclude the # DT_RUNPATH tag from executables and libraries. But doing so # requires that you compile everything twice, which is a pain. if $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath $wl$libdir' _LT_TAGVAR(archive_cmds, $1)='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' else _LT_TAGVAR(ld_shlibs, $1)=no fi ;; esac ;; sunos4*) _LT_TAGVAR(archive_cmds, $1)='$LD -assert pure-text -Bshareable -o $lib $libobjs $deplibs $linker_flags' wlarc= _LT_TAGVAR(hardcode_direct, $1)=yes _LT_TAGVAR(hardcode_shlibpath_var, $1)=no ;; *) if $LD --help 2>&1 | $GREP ': supported targets:.* elf' > /dev/null; then _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' else _LT_TAGVAR(ld_shlibs, $1)=no fi ;; esac if test no = "$_LT_TAGVAR(ld_shlibs, $1)"; then runpath_var= _LT_TAGVAR(hardcode_libdir_flag_spec, $1)= _LT_TAGVAR(export_dynamic_flag_spec, $1)= _LT_TAGVAR(whole_archive_flag_spec, $1)= fi else # PORTME fill in a description of your system's linker (not GNU ld) case $host_os in aix3*) _LT_TAGVAR(allow_undefined_flag, $1)=unsupported _LT_TAGVAR(always_export_symbols, $1)=yes _LT_TAGVAR(archive_expsym_cmds, $1)='$LD -o $output_objdir/$soname $libobjs $deplibs $linker_flags -bE:$export_symbols -T512 -H512 -bM:SRE~$AR $AR_FLAGS $lib $output_objdir/$soname' # Note: this linker hardcodes the directories in LIBPATH if there # are no directories specified by -L. _LT_TAGVAR(hardcode_minus_L, $1)=yes if test yes = "$GCC" && test -z "$lt_prog_compiler_static"; then # Neither direct hardcoding nor static linking is supported with a # broken collect2. _LT_TAGVAR(hardcode_direct, $1)=unsupported fi ;; aix[[4-9]]*) if test ia64 = "$host_cpu"; then # On IA64, the linker does run time linking by default, so we don't # have to do anything special. aix_use_runtimelinking=no exp_sym_flag='-Bexport' no_entry_flag= else # If we're using GNU nm, then we don't want the "-C" option. # -C means demangle to GNU nm, but means don't demangle to AIX nm. # Without the "-l" option, or with the "-B" option, AIX nm treats # weak defined symbols like other global defined symbols, whereas # GNU nm marks them as "W". # While the 'weak' keyword is ignored in the Export File, we need # it in the Import File for the 'aix-soname' feature, so we have # to replace the "-B" option with "-P" for AIX nm. if $NM -V 2>&1 | $GREP 'GNU' > /dev/null; then _LT_TAGVAR(export_symbols_cmds, $1)='$NM -Bpg $libobjs $convenience | awk '\''{ if (((\$ 2 == "T") || (\$ 2 == "D") || (\$ 2 == "B") || (\$ 2 == "W")) && ([substr](\$ 3,1,1) != ".")) { if (\$ 2 == "W") { print \$ 3 " weak" } else { print \$ 3 } } }'\'' | sort -u > $export_symbols' else _LT_TAGVAR(export_symbols_cmds, $1)='`func_echo_all $NM | $SED -e '\''s/B\([[^B]]*\)$/P\1/'\''` -PCpgl $libobjs $convenience | awk '\''{ if (((\$ 2 == "T") || (\$ 2 == "D") || (\$ 2 == "B") || (\$ 2 == "L") || (\$ 2 == "W") || (\$ 2 == "V") || (\$ 2 == "Z")) && ([substr](\$ 1,1,1) != ".")) { if ((\$ 2 == "W") || (\$ 2 == "V") || (\$ 2 == "Z")) { print \$ 1 " weak" } else { print \$ 1 } } }'\'' | sort -u > $export_symbols' fi aix_use_runtimelinking=no # Test if we are trying to use run time linking or normal # AIX style linking. If -brtl is somewhere in LDFLAGS, we # have runtime linking enabled, and use it for executables. # For shared libraries, we enable/disable runtime linking # depending on the kind of the shared library created - # when "with_aix_soname,aix_use_runtimelinking" is: # "aix,no" lib.a(lib.so.V) shared, rtl:no, for executables # "aix,yes" lib.so shared, rtl:yes, for executables # lib.a static archive # "both,no" lib.so.V(shr.o) shared, rtl:yes # lib.a(lib.so.V) shared, rtl:no, for executables # "both,yes" lib.so.V(shr.o) shared, rtl:yes, for executables # lib.a(lib.so.V) shared, rtl:no # "svr4,*" lib.so.V(shr.o) shared, rtl:yes, for executables # lib.a static archive case $host_os in aix4.[[23]]|aix4.[[23]].*|aix[[5-9]]*) for ld_flag in $LDFLAGS; do if (test x-brtl = "x$ld_flag" || test x-Wl,-brtl = "x$ld_flag"); then aix_use_runtimelinking=yes break fi done if test svr4,no = "$with_aix_soname,$aix_use_runtimelinking"; then # With aix-soname=svr4, we create the lib.so.V shared archives only, # so we don't have lib.a shared libs to link our executables. # We have to force runtime linking in this case. aix_use_runtimelinking=yes LDFLAGS="$LDFLAGS -Wl,-brtl" fi ;; esac exp_sym_flag='-bexport' no_entry_flag='-bnoentry' fi # When large executables or shared objects are built, AIX ld can # have problems creating the table of contents. If linking a library # or program results in "error TOC overflow" add -mminimal-toc to # CXXFLAGS/CFLAGS for g++/gcc. In the cases where that is not # enough to fix the problem, add -Wl,-bbigtoc to LDFLAGS. _LT_TAGVAR(archive_cmds, $1)='' _LT_TAGVAR(hardcode_direct, $1)=yes _LT_TAGVAR(hardcode_direct_absolute, $1)=yes _LT_TAGVAR(hardcode_libdir_separator, $1)=':' _LT_TAGVAR(link_all_deplibs, $1)=yes _LT_TAGVAR(file_list_spec, $1)='$wl-f,' case $with_aix_soname,$aix_use_runtimelinking in aix,*) ;; # traditional, no import file svr4,* | *,yes) # use import file # The Import File defines what to hardcode. _LT_TAGVAR(hardcode_direct, $1)=no _LT_TAGVAR(hardcode_direct_absolute, $1)=no ;; esac if test yes = "$GCC"; then case $host_os in aix4.[[012]]|aix4.[[012]].*) # We only want to do this on AIX 4.2 and lower, the check # below for broken collect2 doesn't work under 4.3+ collect2name=`$CC -print-prog-name=collect2` if test -f "$collect2name" && strings "$collect2name" | $GREP resolve_lib_name >/dev/null then # We have reworked collect2 : else # We have old collect2 _LT_TAGVAR(hardcode_direct, $1)=unsupported # It fails to find uninstalled libraries when the uninstalled # path is not listed in the libpath. Setting hardcode_minus_L # to unsupported forces relinking _LT_TAGVAR(hardcode_minus_L, $1)=yes _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-L$libdir' _LT_TAGVAR(hardcode_libdir_separator, $1)= fi ;; esac shared_flag='-shared' if test yes = "$aix_use_runtimelinking"; then shared_flag="$shared_flag "'$wl-G' fi # Need to ensure runtime linking is disabled for the traditional # shared library, or the linker may eventually find shared libraries # /with/ Import File - we do not want to mix them. shared_flag_aix='-shared' shared_flag_svr4='-shared $wl-G' else # not using gcc if test ia64 = "$host_cpu"; then # VisualAge C++, Version 5.5 for AIX 5L for IA-64, Beta 3 Release # chokes on -Wl,-G. The following line is correct: shared_flag='-G' else if test yes = "$aix_use_runtimelinking"; then shared_flag='$wl-G' else shared_flag='$wl-bM:SRE' fi shared_flag_aix='$wl-bM:SRE' shared_flag_svr4='$wl-G' fi fi _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl-bexpall' # It seems that -bexpall does not export symbols beginning with # underscore (_), so it is better to generate a list of symbols to export. _LT_TAGVAR(always_export_symbols, $1)=yes if test aix,yes = "$with_aix_soname,$aix_use_runtimelinking"; then # Warning - without using the other runtime loading flags (-brtl), # -berok will link without error, but may produce a broken library. _LT_TAGVAR(allow_undefined_flag, $1)='-berok' # Determine the default libpath from the value encoded in an # empty executable. _LT_SYS_MODULE_PATH_AIX([$1]) _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-blibpath:$libdir:'"$aix_libpath" _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -o $output_objdir/$soname $libobjs $deplibs $wl'$no_entry_flag' $compiler_flags `if test -n "$allow_undefined_flag"; then func_echo_all "$wl$allow_undefined_flag"; else :; fi` $wl'$exp_sym_flag:\$export_symbols' '$shared_flag else if test ia64 = "$host_cpu"; then _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-R $libdir:/usr/lib:/lib' _LT_TAGVAR(allow_undefined_flag, $1)="-z nodefs" _LT_TAGVAR(archive_expsym_cmds, $1)="\$CC $shared_flag"' -o $output_objdir/$soname $libobjs $deplibs '"\$wl$no_entry_flag"' $compiler_flags $wl$allow_undefined_flag '"\$wl$exp_sym_flag:\$export_symbols" else # Determine the default libpath from the value encoded in an # empty executable. _LT_SYS_MODULE_PATH_AIX([$1]) _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-blibpath:$libdir:'"$aix_libpath" # Warning - without using the other run time loading flags, # -berok will link without error, but may produce a broken library. _LT_TAGVAR(no_undefined_flag, $1)=' $wl-bernotok' _LT_TAGVAR(allow_undefined_flag, $1)=' $wl-berok' if test yes = "$with_gnu_ld"; then # We only use this code for GNU lds that support --whole-archive. _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive$convenience $wl--no-whole-archive' else # Exported symbols can be pulled into shared objects from archives _LT_TAGVAR(whole_archive_flag_spec, $1)='$convenience' fi _LT_TAGVAR(archive_cmds_need_lc, $1)=yes _LT_TAGVAR(archive_expsym_cmds, $1)='$RM -r $output_objdir/$realname.d~$MKDIR $output_objdir/$realname.d' # -brtl affects multiple linker settings, -berok does not and is overridden later compiler_flags_filtered='`func_echo_all "$compiler_flags " | $SED -e "s%-brtl\\([[, ]]\\)%-berok\\1%g"`' if test svr4 != "$with_aix_soname"; then # This is similar to how AIX traditionally builds its shared libraries. _LT_TAGVAR(archive_expsym_cmds, $1)="$_LT_TAGVAR(archive_expsym_cmds, $1)"'~$CC '$shared_flag_aix' -o $output_objdir/$realname.d/$soname $libobjs $deplibs $wl-bnoentry '$compiler_flags_filtered'$wl-bE:$export_symbols$allow_undefined_flag~$AR $AR_FLAGS $output_objdir/$libname$release.a $output_objdir/$realname.d/$soname' fi if test aix != "$with_aix_soname"; then _LT_TAGVAR(archive_expsym_cmds, $1)="$_LT_TAGVAR(archive_expsym_cmds, $1)"'~$CC '$shared_flag_svr4' -o $output_objdir/$realname.d/$shared_archive_member_spec.o $libobjs $deplibs $wl-bnoentry '$compiler_flags_filtered'$wl-bE:$export_symbols$allow_undefined_flag~$STRIP -e $output_objdir/$realname.d/$shared_archive_member_spec.o~( func_echo_all "#! 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solaris*) _LT_TAGVAR(no_undefined_flag, $1)=' -z defs' if test yes = "$GCC"; then wlarc='$wl' _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $wl-z ${wl}text $wl-h $wl$soname -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $CC -shared $pic_flag $wl-z ${wl}text $wl-M $wl$lib.exp $wl-h $wl$soname -o $lib $libobjs $deplibs $compiler_flags~$RM $lib.exp' else case `$CC -V 2>&1` in *"Compilers 5.0"*) wlarc='' _LT_TAGVAR(archive_cmds, $1)='$LD -G$allow_undefined_flag -h $soname -o $lib $libobjs $deplibs $linker_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $LD -G$allow_undefined_flag -M $lib.exp -h $soname -o $lib $libobjs $deplibs $linker_flags~$RM $lib.exp' ;; *) wlarc='$wl' _LT_TAGVAR(archive_cmds, $1)='$CC -G$allow_undefined_flag -h $soname -o $lib $libobjs $deplibs $compiler_flags' _LT_TAGVAR(archive_expsym_cmds, $1)='echo "{ global:" > $lib.exp~cat $export_symbols | $SED -e "s/\(.*\)/\1;/" >> $lib.exp~echo "local: *; };" >> $lib.exp~ $CC -G$allow_undefined_flag -M $lib.exp -h $soname -o $lib $libobjs $deplibs $compiler_flags~$RM $lib.exp' ;; esac fi _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-R$libdir' _LT_TAGVAR(hardcode_shlibpath_var, $1)=no case $host_os in solaris2.[[0-5]] | solaris2.[[0-5]].*) ;; *) # The compiler driver will combine and reorder linker options, # but understands '-z linker_flag'. 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(KAI) C++ Compiler # KCC will only create a shared library if the output file # ends with ".so" (or ".sl" for HP-UX), so rename the library # to its proper name (with version) after linking. _LT_TAGVAR(archive_cmds, $1)='tempext=`echo $shared_ext | $SED -e '\''s/\([[^()0-9A-Za-z{}]]\)/\\\\\1/g'\''`; templib=`echo $lib | $SED -e "s/\$tempext\..*/.so/"`; $CC $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags --soname $soname -o \$templib; mv \$templib $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='tempext=`echo $shared_ext | $SED -e '\''s/\([[^()0-9A-Za-z{}]]\)/\\\\\1/g'\''`; templib=`echo $lib | $SED -e "s/\$tempext\..*/.so/"`; $CC $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags --soname $soname -o \$templib $wl-retain-symbols-file,$export_symbols; mv \$templib $lib' # Commands to make compiler produce verbose output that lists # what "hidden" libraries, object files and flags are used when # linking a shared library. # # There doesn't appear to be a way to prevent this compiler from # explicitly linking system object files so we need to strip them # from the output so that they don't get included in the library # dependencies. output_verbose_link_cmd='templist=`$CC $CFLAGS -v conftest.$objext -o libconftest$shared_ext 2>&1 | $GREP "ld"`; rm -f libconftest$shared_ext; list= ; for z in $templist; do case $z in conftest.$objext) list="$list $z";; *.$objext);; *) list="$list $z";;esac; done; func_echo_all "$list"' _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath,$libdir' _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl--export-dynamic' # Archives containing C++ object files must be created using # "CC -Bstatic", where "CC" is the KAI C++ compiler. _LT_TAGVAR(old_archive_cmds, $1)='$CC -Bstatic -o $oldlib $oldobjs' ;; icpc* | ecpc* ) # Intel C++ with_gnu_ld=yes # version 8.0 and above of icpc choke on multiply defined symbols # if we add $predep_objects and $postdep_objects, however 7.1 and # earlier do not add the objects themselves. case `$CC -V 2>&1` in *"Version 7."*) _LT_TAGVAR(archive_cmds, $1)='$CC -shared $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; *) # Version 8.0 or newer tmp_idyn= case $host_cpu in ia64*) tmp_idyn=' -i_dynamic';; esac _LT_TAGVAR(archive_cmds, $1)='$CC -shared'"$tmp_idyn"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared'"$tmp_idyn"' $libobjs $deplibs $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; esac _LT_TAGVAR(archive_cmds_need_lc, $1)=no _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl-rpath,$libdir' _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl--export-dynamic' _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive$convenience $wl--no-whole-archive' ;; pgCC* | pgcpp*) # Portland Group C++ compiler case `$CC -V` in *pgCC\ [[1-5]].* | *pgcpp\ [[1-5]].*) _LT_TAGVAR(prelink_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $objs $libobjs $compile_deplibs~ compile_command="$compile_command `find $tpldir -name \*.o | sort | $NL2SP`"' _LT_TAGVAR(old_archive_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $oldobjs$old_deplibs~ $AR $AR_FLAGS $oldlib$oldobjs$old_deplibs `find $tpldir -name \*.o | sort | $NL2SP`~ $RANLIB $oldlib' _LT_TAGVAR(archive_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $predep_objects $libobjs $deplibs $convenience $postdep_objects~ $CC -shared $pic_flag $predep_objects $libobjs $deplibs `find $tpldir -name \*.o | sort | $NL2SP` $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='tpldir=Template.dir~ rm -rf $tpldir~ $CC --prelink_objects --instantiation_dir $tpldir $predep_objects $libobjs $deplibs $convenience $postdep_objects~ $CC -shared $pic_flag $predep_objects $libobjs $deplibs `find $tpldir -name \*.o | sort | $NL2SP` $postdep_objects $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; *) # Version 6 and above use weak symbols _LT_TAGVAR(archive_cmds, $1)='$CC -shared $pic_flag $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $pic_flag $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname $wl-retain-symbols-file $wl$export_symbols -o $lib' ;; esac _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='$wl--rpath $wl$libdir' _LT_TAGVAR(export_dynamic_flag_spec, $1)='$wl--export-dynamic' _LT_TAGVAR(whole_archive_flag_spec, $1)='$wl--whole-archive`for conv in $convenience\"\"; do test -n \"$conv\" && new_convenience=\"$new_convenience,$conv\"; done; func_echo_all \"$new_convenience\"` $wl--no-whole-archive' ;; cxx*) # Compaq C++ _LT_TAGVAR(archive_cmds, $1)='$CC -shared $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib' _LT_TAGVAR(archive_expsym_cmds, $1)='$CC -shared $predep_objects $libobjs $deplibs $postdep_objects $compiler_flags $wl-soname $wl$soname -o $lib $wl-retain-symbols-file $wl$export_symbols' runpath_var=LD_RUN_PATH _LT_TAGVAR(hardcode_libdir_flag_spec, $1)='-rpath $libdir' _LT_TAGVAR(hardcode_libdir_separator, $1)=: # Commands to make compiler produce verbose output that lists # what "hidden" libraries, object files and flags are used when # linking a shared library. # # There doesn't appear to be a way to prevent this compiler from # explicitly linking system object files so we need to strip them # from the output so that they don't get included in the library # dependencies. output_verbose_link_cmd='templist=`$CC -shared $CFLAGS -v conftest.$objext 2>&1 | $GREP "ld"`; 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The basic assumption is that dnl a user will want packages to use other packages he previously installed dnl with the same --prefix option. dnl This macro is not needed if only AC_LIB_LINKFLAGS is used to locate dnl libraries, but is otherwise very convenient. AC_DEFUN([AC_LIB_PREFIX], [ AC_BEFORE([$0], [AC_LIB_LINKFLAGS]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AC_LIB_PREPARE_MULTILIB]) AC_REQUIRE([AC_LIB_PREPARE_PREFIX]) dnl By default, look in $includedir and $libdir. use_additional=yes AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) AC_LIB_ARG_WITH([lib-prefix], [ --with-lib-prefix[=DIR] search for libraries in DIR/include and DIR/lib --without-lib-prefix don't search for libraries in includedir and libdir], [ if test "X$withval" = "Xno"; then use_additional=no else if test "X$withval" = "X"; then AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) else additional_includedir="$withval/include" additional_libdir="$withval/$acl_libdirstem" fi fi ]) if test $use_additional = yes; then dnl Potentially add $additional_includedir to $CPPFLAGS. dnl But don't add it dnl 1. if it's the standard /usr/include, dnl 2. if it's already present in $CPPFLAGS, dnl 3. if it's /usr/local/include and we are using GCC on Linux, dnl 4. if it doesn't exist as a directory. if test "X$additional_includedir" != "X/usr/include"; then haveit= for x in $CPPFLAGS; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-I$additional_includedir"; then haveit=yes break fi done if test -z "$haveit"; then if test "X$additional_includedir" = "X/usr/local/include"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then if test -d "$additional_includedir"; then dnl Really add $additional_includedir to $CPPFLAGS. CPPFLAGS="${CPPFLAGS}${CPPFLAGS:+ }-I$additional_includedir" fi fi fi fi dnl Potentially add $additional_libdir to $LDFLAGS. dnl But don't add it dnl 1. if it's the standard /usr/lib, dnl 2. if it's already present in $LDFLAGS, dnl 3. if it's /usr/local/lib and we are using GCC on Linux, dnl 4. if it doesn't exist as a directory. if test "X$additional_libdir" != "X/usr/$acl_libdirstem"; then haveit= for x in $LDFLAGS; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test "X$additional_libdir" = "X/usr/local/$acl_libdirstem"; then if test -n "$GCC"; then case $host_os in linux*) haveit=yes;; esac fi fi if test -z "$haveit"; then if test -d "$additional_libdir"; then dnl Really add $additional_libdir to $LDFLAGS. LDFLAGS="${LDFLAGS}${LDFLAGS:+ }-L$additional_libdir" fi fi fi fi fi ]) dnl AC_LIB_PREPARE_PREFIX creates variables acl_final_prefix, dnl acl_final_exec_prefix, containing the values to which $prefix and dnl $exec_prefix will expand at the end of the configure script. AC_DEFUN([AC_LIB_PREPARE_PREFIX], [ dnl Unfortunately, prefix and exec_prefix get only finally determined dnl at the end of configure. if test "X$prefix" = "XNONE"; then acl_final_prefix="$ac_default_prefix" else acl_final_prefix="$prefix" fi if test "X$exec_prefix" = "XNONE"; then acl_final_exec_prefix='${prefix}' else acl_final_exec_prefix="$exec_prefix" fi acl_save_prefix="$prefix" prefix="$acl_final_prefix" eval acl_final_exec_prefix=\"$acl_final_exec_prefix\" prefix="$acl_save_prefix" ]) dnl AC_LIB_WITH_FINAL_PREFIX([statement]) evaluates statement, with the dnl variables prefix and exec_prefix bound to the values they will have dnl at the end of the configure script. AC_DEFUN([AC_LIB_WITH_FINAL_PREFIX], [ acl_save_prefix="$prefix" prefix="$acl_final_prefix" acl_save_exec_prefix="$exec_prefix" exec_prefix="$acl_final_exec_prefix" $1 exec_prefix="$acl_save_exec_prefix" prefix="$acl_save_prefix" ]) dnl AC_LIB_PREPARE_MULTILIB creates dnl - a variable acl_libdirstem, containing the basename of the libdir, either dnl "lib" or "lib64" or "lib/64", dnl - a variable acl_libdirstem2, as a secondary possible value for dnl acl_libdirstem, either the same as acl_libdirstem or "lib/sparcv9" or dnl "lib/amd64". AC_DEFUN([AC_LIB_PREPARE_MULTILIB], [ dnl There is no formal standard regarding lib and lib64. dnl On glibc systems, the current practice is that on a system supporting dnl 32-bit and 64-bit instruction sets or ABIs, 64-bit libraries go under dnl $prefix/lib64 and 32-bit libraries go under $prefix/lib. We determine dnl the compiler's default mode by looking at the compiler's library search dnl path. 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AC_CACHE_CHECK([for the common suffixes of directories in the library search path], [acl_cv_libdirstems], [acl_libdirstem=lib acl_libdirstem2= case "$host_os" in solaris*) dnl See Solaris 10 Software Developer Collection > Solaris 64-bit Developer's Guide > The Development Environment dnl . dnl "Portable Makefiles should refer to any library directories using the 64 symbolic link." dnl But we want to recognize the sparcv9 or amd64 subdirectory also if the dnl symlink is missing, so we set acl_libdirstem2 too. AC_CACHE_CHECK([for 64-bit host], [gl_cv_solaris_64bit], [AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#ifdef _LP64 int ok; #else error fail #endif ]])], [gl_cv_solaris_64bit=yes], [gl_cv_solaris_64bit=no]) ]) if test $gl_cv_solaris_64bit = yes; then acl_libdirstem=lib/64 case "$host_cpu" in sparc*) acl_libdirstem2=lib/sparcv9 ;; i*86 | x86_64) acl_libdirstem2=lib/amd64 ;; esac fi ;; *) dnl If $CC generates code for a 32-bit ABI, the libraries are dnl surely under $prefix/lib, not $prefix/lib64. case "$gl_cv_host_cpu_c_abi" in i386 | arm | armhf | arm64-ilp32 | hppa | ia64-ilp32 | mips | mipsn32 | powerpc | s390 | sparc) ;; *) # x86_64 | arm64 | hppa64 | ia64 | mips64 | powerpc64* | s390x | sparc64 | ... dnl The result is a property of the system. However, non-system dnl compilers sometimes have odd library search paths. Therefore dnl prefer asking /usr/bin/gcc, if available, rather than $CC. searchpath=`(if test -f /usr/bin/gcc \ && LC_ALL=C /usr/bin/gcc -print-search-dirs >/dev/null 2>/dev/null; then \ LC_ALL=C /usr/bin/gcc -print-search-dirs; \ else \ LC_ALL=C $CC -print-search-dirs; \ fi) 2>/dev/null \ | sed -n -e 's,^libraries: ,,p' | sed -e 's,^=,,'` if test -n "$searchpath"; then acl_save_IFS="${IFS= }"; IFS=":" for searchdir in $searchpath; do if test -d "$searchdir"; then case "$searchdir" in */lib64/ | */lib64 ) acl_libdirstem=lib64 ;; */../ | */.. ) # Better ignore directories of this form. They are misleading. ;; *) searchdir=`cd "$searchdir" && pwd` case "$searchdir" in */lib64 ) acl_libdirstem=lib64 ;; esac ;; esac fi done IFS="$acl_save_IFS" fi ;; esac ;; esac test -n "$acl_libdirstem2" || acl_libdirstem2="$acl_libdirstem" acl_cv_libdirstems="$acl_libdirstem,$acl_libdirstem2" ]) # Decompose acl_cv_libdirstems into acl_libdirstem and acl_libdirstem2. acl_libdirstem=`echo "$acl_cv_libdirstems" | sed -e 's/,.*//'` acl_libdirstem2=`echo "$acl_cv_libdirstems" | sed -e '/,/s/.*,//'` ]) gnuastro-0.5/bootstrapped/m4/lib-link.m40000644000175000017500000010044313217200022015121 00000000000000# lib-link.m4 serial 26 (gettext-0.18.2) dnl Copyright (C) 2001-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_PREREQ([2.54]) dnl AC_LIB_LINKFLAGS(name [, dependencies]) searches for libname and dnl the libraries corresponding to explicit and implicit dependencies. dnl Sets and AC_SUBSTs the LIB${NAME} and LTLIB${NAME} variables and dnl augments the CPPFLAGS variable. dnl Sets and AC_SUBSTs the LIB${NAME}_PREFIX variable to nonempty if libname dnl was found in ${LIB${NAME}_PREFIX}/$acl_libdirstem. AC_DEFUN([AC_LIB_LINKFLAGS], [ AC_REQUIRE([AC_LIB_PREPARE_PREFIX]) AC_REQUIRE([AC_LIB_RPATH]) pushdef([Name],[m4_translit([$1],[./+-], [____])]) pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) AC_CACHE_CHECK([how to link with lib[]$1], [ac_cv_lib[]Name[]_libs], [ AC_LIB_LINKFLAGS_BODY([$1], [$2]) ac_cv_lib[]Name[]_libs="$LIB[]NAME" ac_cv_lib[]Name[]_ltlibs="$LTLIB[]NAME" ac_cv_lib[]Name[]_cppflags="$INC[]NAME" ac_cv_lib[]Name[]_prefix="$LIB[]NAME[]_PREFIX" ]) LIB[]NAME="$ac_cv_lib[]Name[]_libs" LTLIB[]NAME="$ac_cv_lib[]Name[]_ltlibs" INC[]NAME="$ac_cv_lib[]Name[]_cppflags" LIB[]NAME[]_PREFIX="$ac_cv_lib[]Name[]_prefix" AC_LIB_APPENDTOVAR([CPPFLAGS], [$INC]NAME) AC_SUBST([LIB]NAME) AC_SUBST([LTLIB]NAME) AC_SUBST([LIB]NAME[_PREFIX]) dnl Also set HAVE_LIB[]NAME so that AC_LIB_HAVE_LINKFLAGS can reuse the dnl results of this search when this library appears as a dependency. HAVE_LIB[]NAME=yes popdef([NAME]) popdef([Name]) ]) dnl AC_LIB_HAVE_LINKFLAGS(name, dependencies, includes, testcode, [missing-message]) dnl searches for libname and the libraries corresponding to explicit and dnl implicit dependencies, together with the specified include files and dnl the ability to compile and link the specified testcode. The missing-message dnl defaults to 'no' and may contain additional hints for the user. dnl If found, it sets and AC_SUBSTs HAVE_LIB${NAME}=yes and the LIB${NAME} dnl and LTLIB${NAME} variables and augments the CPPFLAGS variable, and dnl #defines HAVE_LIB${NAME} to 1. Otherwise, it sets and AC_SUBSTs dnl HAVE_LIB${NAME}=no and LIB${NAME} and LTLIB${NAME} to empty. dnl Sets and AC_SUBSTs the LIB${NAME}_PREFIX variable to nonempty if libname dnl was found in ${LIB${NAME}_PREFIX}/$acl_libdirstem. AC_DEFUN([AC_LIB_HAVE_LINKFLAGS], [ AC_REQUIRE([AC_LIB_PREPARE_PREFIX]) AC_REQUIRE([AC_LIB_RPATH]) pushdef([Name],[m4_translit([$1],[./+-], [____])]) pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) dnl Search for lib[]Name and define LIB[]NAME, LTLIB[]NAME and INC[]NAME dnl accordingly. AC_LIB_LINKFLAGS_BODY([$1], [$2]) dnl Add $INC[]NAME to CPPFLAGS before performing the following checks, dnl because if the user has installed lib[]Name and not disabled its use dnl via --without-lib[]Name-prefix, he wants to use it. ac_save_CPPFLAGS="$CPPFLAGS" AC_LIB_APPENDTOVAR([CPPFLAGS], [$INC]NAME) AC_CACHE_CHECK([for lib[]$1], [ac_cv_lib[]Name], [ ac_save_LIBS="$LIBS" dnl If $LIB[]NAME contains some -l options, add it to the end of LIBS, dnl because these -l options might require -L options that are present in dnl LIBS. -l options benefit only from the -L options listed before it. dnl Otherwise, add it to the front of LIBS, because it may be a static dnl library that depends on another static library that is present in LIBS. dnl Static libraries benefit only from the static libraries listed after dnl it. case " $LIB[]NAME" in *" -l"*) LIBS="$LIBS $LIB[]NAME" ;; *) LIBS="$LIB[]NAME $LIBS" ;; esac AC_LINK_IFELSE( [AC_LANG_PROGRAM([[$3]], [[$4]])], [ac_cv_lib[]Name=yes], [ac_cv_lib[]Name='m4_if([$5], [], [no], [[$5]])']) LIBS="$ac_save_LIBS" ]) if test "$ac_cv_lib[]Name" = yes; then HAVE_LIB[]NAME=yes AC_DEFINE([HAVE_LIB]NAME, 1, [Define if you have the lib][$1 library.]) AC_MSG_CHECKING([how to link with lib[]$1]) AC_MSG_RESULT([$LIB[]NAME]) else HAVE_LIB[]NAME=no dnl If $LIB[]NAME didn't lead to a usable library, we don't need dnl $INC[]NAME either. CPPFLAGS="$ac_save_CPPFLAGS" LIB[]NAME= LTLIB[]NAME= LIB[]NAME[]_PREFIX= fi AC_SUBST([HAVE_LIB]NAME) AC_SUBST([LIB]NAME) AC_SUBST([LTLIB]NAME) AC_SUBST([LIB]NAME[_PREFIX]) popdef([NAME]) popdef([Name]) ]) dnl Determine the platform dependent parameters needed to use rpath: dnl acl_libext, dnl acl_shlibext, dnl acl_libname_spec, dnl acl_library_names_spec, dnl acl_hardcode_libdir_flag_spec, dnl acl_hardcode_libdir_separator, dnl acl_hardcode_direct, dnl acl_hardcode_minus_L. AC_DEFUN([AC_LIB_RPATH], [ dnl Tell automake >= 1.10 to complain if config.rpath is missing. m4_ifdef([AC_REQUIRE_AUX_FILE], [AC_REQUIRE_AUX_FILE([config.rpath])]) AC_REQUIRE([AC_PROG_CC]) dnl we use $CC, $GCC, $LDFLAGS AC_REQUIRE([AC_LIB_PROG_LD]) dnl we use $LD, $with_gnu_ld AC_REQUIRE([AC_CANONICAL_HOST]) dnl we use $host AC_REQUIRE([AC_CONFIG_AUX_DIR_DEFAULT]) dnl we use $ac_aux_dir AC_CACHE_CHECK([for shared library run path origin], [acl_cv_rpath], [ CC="$CC" GCC="$GCC" LDFLAGS="$LDFLAGS" LD="$LD" with_gnu_ld="$with_gnu_ld" \ ${CONFIG_SHELL-/bin/sh} "$ac_aux_dir/config.rpath" "$host" > conftest.sh . ./conftest.sh rm -f ./conftest.sh acl_cv_rpath=done ]) wl="$acl_cv_wl" acl_libext="$acl_cv_libext" acl_shlibext="$acl_cv_shlibext" acl_libname_spec="$acl_cv_libname_spec" acl_library_names_spec="$acl_cv_library_names_spec" acl_hardcode_libdir_flag_spec="$acl_cv_hardcode_libdir_flag_spec" acl_hardcode_libdir_separator="$acl_cv_hardcode_libdir_separator" acl_hardcode_direct="$acl_cv_hardcode_direct" acl_hardcode_minus_L="$acl_cv_hardcode_minus_L" dnl Determine whether the user wants rpath handling at all. AC_ARG_ENABLE([rpath], [ --disable-rpath do not hardcode runtime library paths], :, enable_rpath=yes) ]) dnl AC_LIB_FROMPACKAGE(name, package) dnl declares that libname comes from the given package. The configure file dnl will then not have a --with-libname-prefix option but a dnl --with-package-prefix option. Several libraries can come from the same dnl package. This declaration must occur before an AC_LIB_LINKFLAGS or similar dnl macro call that searches for libname. AC_DEFUN([AC_LIB_FROMPACKAGE], [ pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) define([acl_frompackage_]NAME, [$2]) popdef([NAME]) pushdef([PACK],[$2]) pushdef([PACKUP],[m4_translit(PACK,[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) define([acl_libsinpackage_]PACKUP, m4_ifdef([acl_libsinpackage_]PACKUP, [m4_defn([acl_libsinpackage_]PACKUP)[, ]],)[lib$1]) popdef([PACKUP]) popdef([PACK]) ]) dnl AC_LIB_LINKFLAGS_BODY(name [, dependencies]) searches for libname and dnl the libraries corresponding to explicit and implicit dependencies. dnl Sets the LIB${NAME}, LTLIB${NAME} and INC${NAME} variables. dnl Also, sets the LIB${NAME}_PREFIX variable to nonempty if libname was found dnl in ${LIB${NAME}_PREFIX}/$acl_libdirstem. AC_DEFUN([AC_LIB_LINKFLAGS_BODY], [ AC_REQUIRE([AC_LIB_PREPARE_MULTILIB]) pushdef([NAME],[m4_translit([$1],[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) pushdef([PACK],[m4_ifdef([acl_frompackage_]NAME, [acl_frompackage_]NAME, lib[$1])]) pushdef([PACKUP],[m4_translit(PACK,[abcdefghijklmnopqrstuvwxyz./+-], [ABCDEFGHIJKLMNOPQRSTUVWXYZ____])]) pushdef([PACKLIBS],[m4_ifdef([acl_frompackage_]NAME, [acl_libsinpackage_]PACKUP, lib[$1])]) dnl Autoconf >= 2.61 supports dots in --with options. pushdef([P_A_C_K],[m4_if(m4_version_compare(m4_defn([m4_PACKAGE_VERSION]),[2.61]),[-1],[m4_translit(PACK,[.],[_])],PACK)]) dnl By default, look in $includedir and $libdir. use_additional=yes AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) AC_ARG_WITH(P_A_C_K[-prefix], [[ --with-]]P_A_C_K[[-prefix[=DIR] search for ]PACKLIBS[ in DIR/include and DIR/lib --without-]]P_A_C_K[[-prefix don't search for ]PACKLIBS[ in includedir and libdir]], [ if test "X$withval" = "Xno"; then use_additional=no else if test "X$withval" = "X"; then AC_LIB_WITH_FINAL_PREFIX([ eval additional_includedir=\"$includedir\" eval additional_libdir=\"$libdir\" ]) else additional_includedir="$withval/include" additional_libdir="$withval/$acl_libdirstem" if test "$acl_libdirstem2" != "$acl_libdirstem" \ && ! test -d "$withval/$acl_libdirstem"; then additional_libdir="$withval/$acl_libdirstem2" fi fi fi ]) dnl Search the library and its dependencies in $additional_libdir and dnl $LDFLAGS. Using breadth-first-seach. LIB[]NAME= LTLIB[]NAME= INC[]NAME= LIB[]NAME[]_PREFIX= dnl HAVE_LIB${NAME} is an indicator that LIB${NAME}, LTLIB${NAME} have been dnl computed. So it has to be reset here. HAVE_LIB[]NAME= rpathdirs= ltrpathdirs= names_already_handled= names_next_round='$1 $2' while test -n "$names_next_round"; do names_this_round="$names_next_round" names_next_round= for name in $names_this_round; do already_handled= for n in $names_already_handled; do if test "$n" = "$name"; then already_handled=yes break fi done if test -z "$already_handled"; then names_already_handled="$names_already_handled $name" dnl See if it was already located by an earlier AC_LIB_LINKFLAGS dnl or AC_LIB_HAVE_LINKFLAGS call. uppername=`echo "$name" | sed -e 'y|abcdefghijklmnopqrstuvwxyz./+-|ABCDEFGHIJKLMNOPQRSTUVWXYZ____|'` eval value=\"\$HAVE_LIB$uppername\" if test -n "$value"; then if test "$value" = yes; then eval value=\"\$LIB$uppername\" test -z "$value" || LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$value" eval value=\"\$LTLIB$uppername\" test -z "$value" || LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }$value" else dnl An earlier call to AC_LIB_HAVE_LINKFLAGS has determined dnl that this library doesn't exist. So just drop it. : fi else dnl Search the library lib$name in $additional_libdir and $LDFLAGS dnl and the already constructed $LIBNAME/$LTLIBNAME. found_dir= found_la= found_so= found_a= eval libname=\"$acl_libname_spec\" # typically: libname=lib$name if test -n "$acl_shlibext"; then shrext=".$acl_shlibext" # typically: shrext=.so else shrext= fi if test $use_additional = yes; then dir="$additional_libdir" dnl The same code as in the loop below: dnl First look for a shared library. if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi dnl Then look for a static library. if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi fi if test "X$found_dir" = "X"; then for x in $LDFLAGS $LTLIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) case "$x" in -L*) dir=`echo "X$x" | sed -e 's/^X-L//'` dnl First look for a shared library. if test -n "$acl_shlibext"; then if test -f "$dir/$libname$shrext"; then found_dir="$dir" found_so="$dir/$libname$shrext" else if test "$acl_library_names_spec" = '$libname$shrext$versuffix'; then ver=`(cd "$dir" && \ for f in "$libname$shrext".*; do echo "$f"; done \ | sed -e "s,^$libname$shrext\\\\.,," \ | sort -t '.' -n -r -k1,1 -k2,2 -k3,3 -k4,4 -k5,5 \ | sed 1q ) 2>/dev/null` if test -n "$ver" && test -f "$dir/$libname$shrext.$ver"; then found_dir="$dir" found_so="$dir/$libname$shrext.$ver" fi else eval library_names=\"$acl_library_names_spec\" for f in $library_names; do if test -f "$dir/$f"; then found_dir="$dir" found_so="$dir/$f" break fi done fi fi fi dnl Then look for a static library. if test "X$found_dir" = "X"; then if test -f "$dir/$libname.$acl_libext"; then found_dir="$dir" found_a="$dir/$libname.$acl_libext" fi fi if test "X$found_dir" != "X"; then if test -f "$dir/$libname.la"; then found_la="$dir/$libname.la" fi fi ;; esac if test "X$found_dir" != "X"; then break fi done fi if test "X$found_dir" != "X"; then dnl Found the library. LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-L$found_dir -l$name" if test "X$found_so" != "X"; then dnl Linking with a shared library. We attempt to hardcode its dnl directory into the executable's runpath, unless it's the dnl standard /usr/lib. if test "$enable_rpath" = no \ || test "X$found_dir" = "X/usr/$acl_libdirstem" \ || test "X$found_dir" = "X/usr/$acl_libdirstem2"; then dnl No hardcoding is needed. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" else dnl Use an explicit option to hardcode DIR into the resulting dnl binary. dnl Potentially add DIR to ltrpathdirs. dnl The ltrpathdirs will be appended to $LTLIBNAME at the end. haveit= for x in $ltrpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $found_dir" fi dnl The hardcoding into $LIBNAME is system dependent. if test "$acl_hardcode_direct" = yes; then dnl Using DIR/libNAME.so during linking hardcodes DIR into the dnl resulting binary. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" else if test -n "$acl_hardcode_libdir_flag_spec" && test "$acl_hardcode_minus_L" = no; then dnl Use an explicit option to hardcode DIR into the resulting dnl binary. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" dnl Potentially add DIR to rpathdirs. dnl The rpathdirs will be appended to $LIBNAME at the end. haveit= for x in $rpathdirs; do if test "X$x" = "X$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $found_dir" fi else dnl Rely on "-L$found_dir". dnl But don't add it if it's already contained in the LDFLAGS dnl or the already constructed $LIBNAME haveit= for x in $LDFLAGS $LIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$found_dir"; then haveit=yes break fi done if test -z "$haveit"; then LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-L$found_dir" fi if test "$acl_hardcode_minus_L" != no; then dnl FIXME: Not sure whether we should use dnl "-L$found_dir -l$name" or "-L$found_dir $found_so" dnl here. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_so" else dnl We cannot use $acl_hardcode_runpath_var and LD_RUN_PATH dnl here, because this doesn't fit in flags passed to the dnl compiler. So give up. No hardcoding. This affects only dnl very old systems. dnl FIXME: Not sure whether we should use dnl "-L$found_dir -l$name" or "-L$found_dir $found_so" dnl here. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-l$name" fi fi fi fi else if test "X$found_a" != "X"; then dnl Linking with a static library. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$found_a" else dnl We shouldn't come here, but anyway it's good to have a dnl fallback. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-L$found_dir -l$name" fi fi dnl Assume the include files are nearby. additional_includedir= case "$found_dir" in */$acl_libdirstem | */$acl_libdirstem/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem/"'*$,,'` if test "$name" = '$1'; then LIB[]NAME[]_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; */$acl_libdirstem2 | */$acl_libdirstem2/) basedir=`echo "X$found_dir" | sed -e 's,^X,,' -e "s,/$acl_libdirstem2/"'*$,,'` if test "$name" = '$1'; then LIB[]NAME[]_PREFIX="$basedir" fi additional_includedir="$basedir/include" ;; esac if test "X$additional_includedir" != "X"; then dnl Potentially add $additional_includedir to $INCNAME. dnl But don't add it dnl 1. if it's the standard /usr/include, dnl 2. if it's /usr/local/include and we are using GCC on Linux, dnl 3. if it's already present in $CPPFLAGS or the already dnl constructed $INCNAME, dnl 4. if it doesn't exist as a directory. if test "X$additional_includedir" != "X/usr/include"; then haveit= if test "X$additional_includedir" = "X/usr/local/include"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then for x in $CPPFLAGS $INC[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-I$additional_includedir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_includedir"; then dnl Really add $additional_includedir to $INCNAME. INC[]NAME="${INC[]NAME}${INC[]NAME:+ }-I$additional_includedir" fi fi fi fi fi dnl Look for dependencies. if test -n "$found_la"; then dnl Read the .la file. It defines the variables dnl dlname, library_names, old_library, dependency_libs, current, dnl age, revision, installed, dlopen, dlpreopen, libdir. save_libdir="$libdir" case "$found_la" in */* | *\\*) . "$found_la" ;; *) . "./$found_la" ;; esac libdir="$save_libdir" dnl We use only dependency_libs. for dep in $dependency_libs; do case "$dep" in -L*) additional_libdir=`echo "X$dep" | sed -e 's/^X-L//'` dnl Potentially add $additional_libdir to $LIBNAME and $LTLIBNAME. dnl But don't add it dnl 1. if it's the standard /usr/lib, dnl 2. if it's /usr/local/lib and we are using GCC on Linux, dnl 3. if it's already present in $LDFLAGS or the already dnl constructed $LIBNAME, dnl 4. if it doesn't exist as a directory. if test "X$additional_libdir" != "X/usr/$acl_libdirstem" \ && test "X$additional_libdir" != "X/usr/$acl_libdirstem2"; then haveit= if test "X$additional_libdir" = "X/usr/local/$acl_libdirstem" \ || test "X$additional_libdir" = "X/usr/local/$acl_libdirstem2"; then if test -n "$GCC"; then case $host_os in linux* | gnu* | k*bsd*-gnu) haveit=yes;; esac fi fi if test -z "$haveit"; then haveit= for x in $LDFLAGS $LIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then dnl Really add $additional_libdir to $LIBNAME. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-L$additional_libdir" fi fi haveit= for x in $LDFLAGS $LTLIB[]NAME; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X-L$additional_libdir"; then haveit=yes break fi done if test -z "$haveit"; then if test -d "$additional_libdir"; then dnl Really add $additional_libdir to $LTLIBNAME. LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-L$additional_libdir" fi fi fi fi ;; -R*) dir=`echo "X$dep" | sed -e 's/^X-R//'` if test "$enable_rpath" != no; then dnl Potentially add DIR to rpathdirs. dnl The rpathdirs will be appended to $LIBNAME at the end. haveit= for x in $rpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then rpathdirs="$rpathdirs $dir" fi dnl Potentially add DIR to ltrpathdirs. dnl The ltrpathdirs will be appended to $LTLIBNAME at the end. haveit= for x in $ltrpathdirs; do if test "X$x" = "X$dir"; then haveit=yes break fi done if test -z "$haveit"; then ltrpathdirs="$ltrpathdirs $dir" fi fi ;; -l*) dnl Handle this in the next round. names_next_round="$names_next_round "`echo "X$dep" | sed -e 's/^X-l//'` ;; *.la) dnl Handle this in the next round. Throw away the .la's dnl directory; it is already contained in a preceding -L dnl option. names_next_round="$names_next_round "`echo "X$dep" | sed -e 's,^X.*/,,' -e 's,^lib,,' -e 's,\.la$,,'` ;; *) dnl Most likely an immediate library name. LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$dep" LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }$dep" ;; esac done fi else dnl Didn't find the library; assume it is in the system directories dnl known to the linker and runtime loader. (All the system dnl directories known to the linker should also be known to the dnl runtime loader, otherwise the system is severely misconfigured.) LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }-l$name" LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-l$name" fi fi fi done done if test "X$rpathdirs" != "X"; then if test -n "$acl_hardcode_libdir_separator"; then dnl Weird platform: only the last -rpath option counts, the user must dnl pass all path elements in one option. We can arrange that for a dnl single library, but not when more than one $LIBNAMEs are used. alldirs= for found_dir in $rpathdirs; do alldirs="${alldirs}${alldirs:+$acl_hardcode_libdir_separator}$found_dir" done dnl Note: acl_hardcode_libdir_flag_spec uses $libdir and $wl. acl_save_libdir="$libdir" libdir="$alldirs" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$flag" else dnl The -rpath options are cumulative. for found_dir in $rpathdirs; do acl_save_libdir="$libdir" libdir="$found_dir" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" LIB[]NAME="${LIB[]NAME}${LIB[]NAME:+ }$flag" done fi fi if test "X$ltrpathdirs" != "X"; then dnl When using libtool, the option that works for both libraries and dnl executables is -R. The -R options are cumulative. for found_dir in $ltrpathdirs; do LTLIB[]NAME="${LTLIB[]NAME}${LTLIB[]NAME:+ }-R$found_dir" done fi popdef([P_A_C_K]) popdef([PACKLIBS]) popdef([PACKUP]) popdef([PACK]) popdef([NAME]) ]) dnl AC_LIB_APPENDTOVAR(VAR, CONTENTS) appends the elements of CONTENTS to VAR, dnl unless already present in VAR. dnl Works only for CPPFLAGS, not for LIB* variables because that sometimes dnl contains two or three consecutive elements that belong together. AC_DEFUN([AC_LIB_APPENDTOVAR], [ for element in [$2]; do haveit= for x in $[$1]; do AC_LIB_WITH_FINAL_PREFIX([eval x=\"$x\"]) if test "X$x" = "X$element"; then haveit=yes break fi done if test -z "$haveit"; then [$1]="${[$1]}${[$1]:+ }$element" fi done ]) dnl For those cases where a variable contains several -L and -l options dnl referring to unknown libraries and directories, this macro determines the dnl necessary additional linker options for the runtime path. dnl AC_LIB_LINKFLAGS_FROM_LIBS([LDADDVAR], [LIBSVALUE], [USE-LIBTOOL]) dnl sets LDADDVAR to linker options needed together with LIBSVALUE. dnl If USE-LIBTOOL evaluates to non-empty, linking with libtool is assumed, dnl otherwise linking without libtool is assumed. AC_DEFUN([AC_LIB_LINKFLAGS_FROM_LIBS], [ AC_REQUIRE([AC_LIB_RPATH]) AC_REQUIRE([AC_LIB_PREPARE_MULTILIB]) $1= if test "$enable_rpath" != no; then if test -n "$acl_hardcode_libdir_flag_spec" && test "$acl_hardcode_minus_L" = no; then dnl Use an explicit option to hardcode directories into the resulting dnl binary. rpathdirs= next= for opt in $2; do if test -n "$next"; then dir="$next" dnl No need to hardcode the standard /usr/lib. if test "X$dir" != "X/usr/$acl_libdirstem" \ && test "X$dir" != "X/usr/$acl_libdirstem2"; then rpathdirs="$rpathdirs $dir" fi next= else case $opt in -L) next=yes ;; -L*) dir=`echo "X$opt" | sed -e 's,^X-L,,'` dnl No need to hardcode the standard /usr/lib. if test "X$dir" != "X/usr/$acl_libdirstem" \ && test "X$dir" != "X/usr/$acl_libdirstem2"; then rpathdirs="$rpathdirs $dir" fi next= ;; *) next= ;; esac fi done if test "X$rpathdirs" != "X"; then if test -n ""$3""; then dnl libtool is used for linking. Use -R options. for dir in $rpathdirs; do $1="${$1}${$1:+ }-R$dir" done else dnl The linker is used for linking directly. if test -n "$acl_hardcode_libdir_separator"; then dnl Weird platform: only the last -rpath option counts, the user dnl must pass all path elements in one option. alldirs= for dir in $rpathdirs; do alldirs="${alldirs}${alldirs:+$acl_hardcode_libdir_separator}$dir" done acl_save_libdir="$libdir" libdir="$alldirs" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" $1="$flag" else dnl The -rpath options are cumulative. for dir in $rpathdirs; do acl_save_libdir="$libdir" libdir="$dir" eval flag=\"$acl_hardcode_libdir_flag_spec\" libdir="$acl_save_libdir" $1="${$1}${$1:+ }$flag" done fi fi fi fi fi AC_SUBST([$1]) ]) gnuastro-0.5/bootstrapped/m4/lib-ld.m40000644000175000017500000001237213217200022014566 00000000000000# lib-ld.m4 serial 9 dnl Copyright (C) 1996-2003, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Subroutines of libtool.m4, dnl with replacements s/_*LT_PATH/AC_LIB_PROG/ and s/lt_/acl_/ to avoid dnl collision with libtool.m4. dnl From libtool-2.4. Sets the variable with_gnu_ld to yes or no. AC_DEFUN([AC_LIB_PROG_LD_GNU], [AC_CACHE_CHECK([if the linker ($LD) is GNU ld], [acl_cv_prog_gnu_ld], [# I'd rather use --version here, but apparently some GNU lds only accept -v. case `$LD -v 2>&1 /dev/null 2>&1 \ && { (PATH='/bin:/bin'; FPATH=$PATH; sh -c :) >/dev/null 2>&1 \ || PATH_SEPARATOR=';' } fi if test -n "$LD"; then AC_MSG_CHECKING([for ld]) elif test "$GCC" = yes; then AC_MSG_CHECKING([for ld used by $CC]) elif test "$with_gnu_ld" = yes; then AC_MSG_CHECKING([for GNU ld]) else AC_MSG_CHECKING([for non-GNU ld]) fi if test -n "$LD"; then # Let the user override the test with a path. : else AC_CACHE_VAL([acl_cv_path_LD], [ acl_cv_path_LD= # Final result of this test ac_prog=ld # Program to search in $PATH if test "$GCC" = yes; then # Check if gcc -print-prog-name=ld gives a path. case $host in *-*-mingw*) # gcc leaves a trailing carriage return which upsets mingw acl_output=`($CC -print-prog-name=ld) 2>&5 | tr -d '\015'` ;; *) acl_output=`($CC -print-prog-name=ld) 2>&5` ;; esac case $acl_output in # Accept absolute paths. [[\\/]]* | ?:[[\\/]]*) re_direlt='/[[^/]][[^/]]*/\.\./' # Canonicalize the pathname of ld acl_output=`echo "$acl_output" | sed 's%\\\\%/%g'` while echo "$acl_output" | grep "$re_direlt" > /dev/null 2>&1; do acl_output=`echo $acl_output | sed "s%$re_direlt%/%"` done # Got the pathname. No search in PATH is needed. acl_cv_path_LD="$acl_output" ac_prog= ;; "") # If it fails, then pretend we aren't using GCC. ;; *) # If it is relative, then search for the first ld in PATH. with_gnu_ld=unknown ;; esac fi if test -n "$ac_prog"; then # Search for $ac_prog in $PATH. acl_save_ifs="$IFS"; IFS=$PATH_SEPARATOR for ac_dir in $PATH; do IFS="$acl_save_ifs" test -z "$ac_dir" && ac_dir=. if test -f "$ac_dir/$ac_prog" || test -f "$ac_dir/$ac_prog$ac_exeext"; then acl_cv_path_LD="$ac_dir/$ac_prog" # Check to see if the program is GNU ld. I'd rather use --version, # but apparently some variants of GNU ld only accept -v. # Break only if it was the GNU/non-GNU ld that we prefer. case `"$acl_cv_path_LD" -v 2>&1 double (*funcptr) (double, int) = ldexp; double x;]], [[return ldexp (x, -1) > 0;]])], [gl_cv_func_ldexp_in_libm=yes], [gl_cv_func_ldexp_in_libm=no]) LIBS="$save_LIBS" ]) if test $gl_cv_func_ldexp_in_libm = yes; then LDEXP_LIBM=-lm fi fi AC_SUBST([LDEXP_LIBM]) ]) dnl Test whether ldexp() can be used without linking with libm. dnl Set gl_cv_func_ldexp_no_libm to 'yes' or 'no' accordingly. AC_DEFUN([gl_CHECK_LDEXP_NO_LIBM], [ AC_CACHE_CHECK([whether ldexp() can be used without linking with libm], [gl_cv_func_ldexp_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM([[#ifndef __NO_MATH_INLINES # define __NO_MATH_INLINES 1 /* for glibc */ #endif #include double (*funcptr) (double, int) = ldexp; double x;]], [[return ldexp (x, -1) > 0;]])], [gl_cv_func_ldexp_no_libm=yes], [gl_cv_func_ldexp_no_libm=no]) ]) ]) gnuastro-0.5/bootstrapped/m4/lcmessage.m40000644000175000017500000000252513217200022015365 00000000000000# lcmessage.m4 serial 7 (gettext-0.18.2) dnl Copyright (C) 1995-2002, 2004-2005, 2008-2014, 2016 Free Software dnl Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl dnl This file can be used in projects which are not available under dnl the GNU General Public License or the GNU Library General Public dnl License but which still want to provide support for the GNU gettext dnl functionality. dnl Please note that the actual code of the GNU gettext library is covered dnl by the GNU Library General Public License, and the rest of the GNU dnl gettext package is covered by the GNU General Public License. dnl They are *not* in the public domain. dnl Authors: dnl Ulrich Drepper , 1995. # Check whether LC_MESSAGES is available in . AC_DEFUN([gt_LC_MESSAGES], [ AC_CACHE_CHECK([for LC_MESSAGES], [gt_cv_val_LC_MESSAGES], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[return LC_MESSAGES]])], [gt_cv_val_LC_MESSAGES=yes], [gt_cv_val_LC_MESSAGES=no])]) if test $gt_cv_val_LC_MESSAGES = yes; then AC_DEFINE([HAVE_LC_MESSAGES], [1], [Define if your file defines LC_MESSAGES.]) fi ]) gnuastro-0.5/bootstrapped/m4/largefile.m40000644000175000017500000001345313217200022015356 00000000000000# Enable large files on systems where this is not the default. # Copyright 1992-1996, 1998-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # The following implementation works around a problem in autoconf <= 2.69; # AC_SYS_LARGEFILE does not configure for large inodes on Mac OS X 10.5, # or configures them incorrectly in some cases. m4_version_prereq([2.70], [] ,[ # _AC_SYS_LARGEFILE_TEST_INCLUDES # ------------------------------- m4_define([_AC_SYS_LARGEFILE_TEST_INCLUDES], [@%:@include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ @%:@define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]];[]dnl ]) # _AC_SYS_LARGEFILE_MACRO_VALUE(C-MACRO, VALUE, # CACHE-VAR, # DESCRIPTION, # PROLOGUE, [FUNCTION-BODY]) # -------------------------------------------------------- m4_define([_AC_SYS_LARGEFILE_MACRO_VALUE], [AC_CACHE_CHECK([for $1 value needed for large files], [$3], [while :; do m4_ifval([$6], [AC_LINK_IFELSE], [AC_COMPILE_IFELSE])( [AC_LANG_PROGRAM([$5], [$6])], [$3=no; break]) m4_ifval([$6], [AC_LINK_IFELSE], [AC_COMPILE_IFELSE])( [AC_LANG_PROGRAM([@%:@define $1 $2 $5], [$6])], [$3=$2; break]) $3=unknown break done]) case $$3 in #( no | unknown) ;; *) AC_DEFINE_UNQUOTED([$1], [$$3], [$4]);; esac rm -rf conftest*[]dnl ])# _AC_SYS_LARGEFILE_MACRO_VALUE # AC_SYS_LARGEFILE # ---------------- # By default, many hosts won't let programs access large files; # one must use special compiler options to get large-file access to work. # For more details about this brain damage please see: # http://www.unix-systems.org/version2/whatsnew/lfs20mar.html AC_DEFUN([AC_SYS_LARGEFILE], [AC_ARG_ENABLE(largefile, [ --disable-largefile omit support for large files]) if test "$enable_largefile" != no; then AC_CACHE_CHECK([for special C compiler options needed for large files], ac_cv_sys_largefile_CC, [ac_cv_sys_largefile_CC=no if test "$GCC" != yes; then ac_save_CC=$CC while :; do # IRIX 6.2 and later do not support large files by default, # so use the C compiler's -n32 option if that helps. AC_LANG_CONFTEST([AC_LANG_PROGRAM([_AC_SYS_LARGEFILE_TEST_INCLUDES])]) AC_COMPILE_IFELSE([], [break]) CC="$CC -n32" AC_COMPILE_IFELSE([], [ac_cv_sys_largefile_CC=' -n32'; break]) break done CC=$ac_save_CC rm -f conftest.$ac_ext fi]) if test "$ac_cv_sys_largefile_CC" != no; then CC=$CC$ac_cv_sys_largefile_CC fi _AC_SYS_LARGEFILE_MACRO_VALUE(_FILE_OFFSET_BITS, 64, ac_cv_sys_file_offset_bits, [Number of bits in a file offset, on hosts where this is settable.], [_AC_SYS_LARGEFILE_TEST_INCLUDES]) if test $ac_cv_sys_file_offset_bits = unknown; then _AC_SYS_LARGEFILE_MACRO_VALUE(_LARGE_FILES, 1, ac_cv_sys_large_files, [Define for large files, on AIX-style hosts.], [_AC_SYS_LARGEFILE_TEST_INCLUDES]) fi AC_DEFINE([_DARWIN_USE_64_BIT_INODE], [1], [Enable large inode numbers on Mac OS X 10.5.]) fi ])# AC_SYS_LARGEFILE ])# m4_version_prereq 2.70 # Enable large files on systems where this is implemented by Gnulib, not by the # system headers. # Set the variables WINDOWS_64_BIT_OFF_T, WINDOWS_64_BIT_ST_SIZE if Gnulib # overrides ensure that off_t or 'struct size.st_size' are 64-bit, respectively. AC_DEFUN([gl_LARGEFILE], [ AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in mingw*) dnl Native Windows. dnl mingw64 defines off_t to a 64-bit type already, if dnl _FILE_OFFSET_BITS=64, which is ensured by AC_SYS_LARGEFILE. AC_CACHE_CHECK([for 64-bit off_t], [gl_cv_type_off_t_64], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int verify_off_t_size[sizeof (off_t) >= 8 ? 1 : -1]; ]], [[]])], [gl_cv_type_off_t_64=yes], [gl_cv_type_off_t_64=no]) ]) if test $gl_cv_type_off_t_64 = no; then WINDOWS_64_BIT_OFF_T=1 else WINDOWS_64_BIT_OFF_T=0 fi dnl Some mingw versions define, if _FILE_OFFSET_BITS=64, 'struct stat' dnl to 'struct _stat32i64' or 'struct _stat64' (depending on dnl _USE_32BIT_TIME_T), which has a 32-bit st_size member. AC_CACHE_CHECK([for 64-bit st_size], [gl_cv_member_st_size_64], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include struct stat buf; int verify_st_size_size[sizeof (buf.st_size) >= 8 ? 1 : -1]; ]], [[]])], [gl_cv_member_st_size_64=yes], [gl_cv_member_st_size_64=no]) ]) if test $gl_cv_member_st_size_64 = no; then WINDOWS_64_BIT_ST_SIZE=1 else WINDOWS_64_BIT_ST_SIZE=0 fi ;; *) dnl Nothing to do on gnulib's side. dnl A 64-bit off_t is dnl - already the default on Mac OS X, FreeBSD, NetBSD, OpenBSD, IRIX, dnl OSF/1, Cygwin, dnl - enabled by _FILE_OFFSET_BITS=64 (ensured by AC_SYS_LARGEFILE) on dnl glibc, HP-UX, Solaris, dnl - enabled by _LARGE_FILES=1 (ensured by AC_SYS_LARGEFILE) on AIX, dnl - impossible to achieve on Minix 3.1.8. WINDOWS_64_BIT_OFF_T=0 WINDOWS_64_BIT_ST_SIZE=0 ;; esac ]) gnuastro-0.5/bootstrapped/m4/langinfo_h.m40000644000175000017500000000672113217200022015530 00000000000000# langinfo_h.m4 serial 7 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LANGINFO_H], [ AC_REQUIRE([gl_LANGINFO_H_DEFAULTS]) dnl Persuade glibc-2.0.6 to define CODESET. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([langinfo.h]) dnl Determine whether exists. It is missing on mingw and BeOS. HAVE_LANGINFO_CODESET=0 HAVE_LANGINFO_T_FMT_AMPM=0 HAVE_LANGINFO_ERA=0 HAVE_LANGINFO_YESEXPR=0 AC_CHECK_HEADERS_ONCE([langinfo.h]) if test $ac_cv_header_langinfo_h = yes; then HAVE_LANGINFO_H=1 dnl Determine what defines. CODESET and ERA etc. are missing dnl on OpenBSD 3.8. T_FMT_AMPM and YESEXPR, NOEXPR are missing on IRIX 5.3. AC_CACHE_CHECK([whether langinfo.h defines CODESET], [gl_cv_header_langinfo_codeset], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = CODESET; ]])], [gl_cv_header_langinfo_codeset=yes], [gl_cv_header_langinfo_codeset=no]) ]) if test $gl_cv_header_langinfo_codeset = yes; then HAVE_LANGINFO_CODESET=1 fi AC_CACHE_CHECK([whether langinfo.h defines T_FMT_AMPM], [gl_cv_header_langinfo_t_fmt_ampm], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = T_FMT_AMPM; ]])], [gl_cv_header_langinfo_t_fmt_ampm=yes], [gl_cv_header_langinfo_t_fmt_ampm=no]) ]) if test $gl_cv_header_langinfo_t_fmt_ampm = yes; then HAVE_LANGINFO_T_FMT_AMPM=1 fi AC_CACHE_CHECK([whether langinfo.h defines ERA], [gl_cv_header_langinfo_era], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = ERA; ]])], [gl_cv_header_langinfo_era=yes], [gl_cv_header_langinfo_era=no]) ]) if test $gl_cv_header_langinfo_era = yes; then HAVE_LANGINFO_ERA=1 fi AC_CACHE_CHECK([whether langinfo.h defines YESEXPR], [gl_cv_header_langinfo_yesexpr], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include int a = YESEXPR; ]])], [gl_cv_header_langinfo_yesexpr=yes], [gl_cv_header_langinfo_yesexpr=no]) ]) if test $gl_cv_header_langinfo_yesexpr = yes; then HAVE_LANGINFO_YESEXPR=1 fi else HAVE_LANGINFO_H=0 fi AC_SUBST([HAVE_LANGINFO_H]) AC_SUBST([HAVE_LANGINFO_CODESET]) AC_SUBST([HAVE_LANGINFO_T_FMT_AMPM]) AC_SUBST([HAVE_LANGINFO_ERA]) AC_SUBST([HAVE_LANGINFO_YESEXPR]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [nl_langinfo]) ]) AC_DEFUN([gl_LANGINFO_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_LANGINFO_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_LANGINFO_H_DEFAULTS], [ GNULIB_NL_LANGINFO=0; AC_SUBST([GNULIB_NL_LANGINFO]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_NL_LANGINFO=1; AC_SUBST([HAVE_NL_LANGINFO]) REPLACE_NL_LANGINFO=0; AC_SUBST([REPLACE_NL_LANGINFO]) ]) gnuastro-0.5/bootstrapped/m4/iswblank.m40000644000175000017500000000234113217200022015230 00000000000000# iswblank.m4 serial 4 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_ISWBLANK], [ AC_REQUIRE([gl_WCTYPE_H_DEFAULTS]) AC_REQUIRE([gl_WCTYPE_H]) dnl Persuade glibc to declare iswblank(). AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_FUNCS_ONCE([iswblank]) AC_CHECK_DECLS([iswblank], , , [[ /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include #include ]]) if test $ac_cv_func_iswblank = no; then HAVE_ISWBLANK=0 if test $ac_cv_have_decl_iswblank = yes; then REPLACE_ISWBLANK=1 fi fi if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then dnl Redefine all of iswcntrl, ..., towupper in . : else if test $HAVE_ISWBLANK = 0 || test $REPLACE_ISWBLANK = 1; then dnl Redefine only iswblank. : fi fi ]) gnuastro-0.5/bootstrapped/m4/isnanl.m40000644000175000017500000001641713217200022014713 00000000000000# isnanl.m4 serial 20 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_ISNANL], [ AC_REQUIRE([gl_MATH_H_DEFAULTS]) ISNANL_LIBM= gl_HAVE_ISNANL_NO_LIBM if test $gl_cv_func_isnanl_no_libm = no; then gl_HAVE_ISNANL_IN_LIBM if test $gl_cv_func_isnanl_in_libm = yes; then ISNANL_LIBM=-lm fi fi dnl The variable gl_func_isnanl set here is used by isnan.m4. if test $gl_cv_func_isnanl_no_libm = yes \ || test $gl_cv_func_isnanl_in_libm = yes; then save_LIBS="$LIBS" LIBS="$LIBS $ISNANL_LIBM" gl_FUNC_ISNANL_WORKS LIBS="$save_LIBS" case "$gl_cv_func_isnanl_works" in *yes) gl_func_isnanl=yes ;; *) gl_func_isnanl=no; ISNANL_LIBM= ;; esac else gl_func_isnanl=no fi if test $gl_func_isnanl != yes; then HAVE_ISNANL=0 fi AC_SUBST([ISNANL_LIBM]) ]) AC_DEFUN([gl_FUNC_ISNANL_NO_LIBM], [ gl_HAVE_ISNANL_NO_LIBM gl_func_isnanl_no_libm=$gl_cv_func_isnanl_no_libm if test $gl_func_isnanl_no_libm = yes; then gl_FUNC_ISNANL_WORKS case "$gl_cv_func_isnanl_works" in *yes) ;; *) gl_func_isnanl_no_libm=no ;; esac fi if test $gl_func_isnanl_no_libm = yes; then AC_DEFINE([HAVE_ISNANL_IN_LIBC], [1], [Define if the isnan(long double) function is available in libc.]) fi ]) dnl Prerequisites of replacement isnanl definition. It does not need -lm. AC_DEFUN([gl_PREREQ_ISNANL], [ gl_LONG_DOUBLE_EXPONENT_LOCATION AC_REQUIRE([gl_LONG_DOUBLE_VS_DOUBLE]) ]) dnl Test whether isnanl() can be used without libm. AC_DEFUN([gl_HAVE_ISNANL_NO_LIBM], [ AC_CACHE_CHECK([whether isnan(long double) can be used without linking with libm], [gl_cv_func_isnanl_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #if __GNUC__ >= 4 # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) #elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) #endif long double x;]], [[return isnanl (x);]])], [gl_cv_func_isnanl_no_libm=yes], [gl_cv_func_isnanl_no_libm=no]) ]) ]) dnl Test whether isnanl() can be used with libm. AC_DEFUN([gl_HAVE_ISNANL_IN_LIBM], [ AC_CACHE_CHECK([whether isnan(long double) can be used with libm], [gl_cv_func_isnanl_in_libm], [ save_LIBS="$LIBS" LIBS="$LIBS -lm" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #if __GNUC__ >= 4 # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) #elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) #endif long double x;]], [[return isnanl (x);]])], [gl_cv_func_isnanl_in_libm=yes], [gl_cv_func_isnanl_in_libm=no]) LIBS="$save_LIBS" ]) ]) dnl Test whether isnanl() recognizes all canonical numbers which are neither dnl finite nor infinite. AC_DEFUN([gl_FUNC_ISNANL_WORKS], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gl_BIGENDIAN]) AC_REQUIRE([gl_LONG_DOUBLE_VS_DOUBLE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([whether isnanl works], [gl_cv_func_isnanl_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #if __GNUC__ >= 4 # undef isnanl # define isnanl(x) __builtin_isnanl ((long double)(x)) #elif defined isnan # undef isnanl # define isnanl(x) isnan ((long double)(x)) #endif #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { unsigned int word[NWORDS]; long double value; } memory_long_double; /* On Irix 6.5, gcc 3.4.3 can't compute compile-time NaN, and needs the runtime type conversion. */ #ifdef __sgi static long double NaNl () { double zero = 0.0; return zero / zero; } #else # define NaNl() (0.0L / 0.0L) #endif int main () { int result = 0; if (!isnanl (NaNl ())) result |= 1; { memory_long_double m; unsigned int i; /* The isnanl function should be immune against changes in the sign bit and in the mantissa bits. The xor operation twiddles a bit that can only be a sign bit or a mantissa bit (since the exponent never extends to bit 31). */ m.value = NaNl (); m.word[NWORDS / 2] ^= (unsigned int) 1 << (sizeof (unsigned int) * CHAR_BIT - 1); for (i = 0; i < NWORDS; i++) m.word[i] |= 1; if (!isnanl (m.value)) result |= 1; } #if ((defined __ia64 && LDBL_MANT_DIG == 64) || (defined __x86_64__ || defined __amd64__) || (defined __i386 || defined __i386__ || defined _I386 || defined _M_IX86 || defined _X86_)) && !HAVE_SAME_LONG_DOUBLE_AS_DOUBLE /* Representation of an 80-bit 'long double' as an initializer for a sequence of 'unsigned int' words. */ # ifdef WORDS_BIGENDIAN # define LDBL80_WORDS(exponent,manthi,mantlo) \ { ((unsigned int) (exponent) << 16) | ((unsigned int) (manthi) >> 16), \ ((unsigned int) (manthi) << 16) | ((unsigned int) (mantlo) >> 16), \ (unsigned int) (mantlo) << 16 \ } # else # define LDBL80_WORDS(exponent,manthi,mantlo) \ { mantlo, manthi, exponent } # endif { /* Quiet NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0xC3333333, 0x00000000) }; if (!isnanl (x.value)) result |= 2; } { /* Signalling NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x83333333, 0x00000000) }; if (!isnanl (x.value)) result |= 2; } /* isnanl should return something even for noncanonical values. */ { /* Pseudo-NaN. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x40000001, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 4; } { /* Pseudo-Infinity. */ static memory_long_double x = { LDBL80_WORDS (0xFFFF, 0x00000000, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 8; } { /* Pseudo-Zero. */ static memory_long_double x = { LDBL80_WORDS (0x4004, 0x00000000, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 16; } { /* Unnormalized number. */ static memory_long_double x = { LDBL80_WORDS (0x4000, 0x63333333, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 32; } { /* Pseudo-Denormal. */ static memory_long_double x = { LDBL80_WORDS (0x0000, 0x83333333, 0x00000000) }; if (isnanl (x.value) && !isnanl (x.value)) result |= 64; } #endif return result; }]])], [gl_cv_func_isnanl_works=yes], [gl_cv_func_isnanl_works=no], [case "$host_os" in mingw*) # Guess yes on mingw, no on MSVC. AC_EGREP_CPP([Known], [ #ifdef __MINGW32__ Known #endif ], [gl_cv_func_isnanl_works="guessing yes"], [gl_cv_func_isnanl_works="guessing no"]) ;; *) gl_cv_func_isnanl_works="guessing yes" ;; esac ]) ]) ]) gnuastro-0.5/bootstrapped/m4/isnanf.m40000644000175000017500000001264313217200022014702 00000000000000# isnanf.m4 serial 15 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Check how to get or define isnanf(). AC_DEFUN([gl_FUNC_ISNANF], [ AC_REQUIRE([gl_MATH_H_DEFAULTS]) ISNANF_LIBM= gl_HAVE_ISNANF_NO_LIBM if test $gl_cv_func_isnanf_no_libm = no; then gl_HAVE_ISNANF_IN_LIBM if test $gl_cv_func_isnanf_in_libm = yes; then ISNANF_LIBM=-lm fi fi dnl The variable gl_func_isnanf set here is used by isnan.m4. if test $gl_cv_func_isnanf_no_libm = yes \ || test $gl_cv_func_isnanf_in_libm = yes; then save_LIBS="$LIBS" LIBS="$LIBS $ISNANF_LIBM" gl_ISNANF_WORKS LIBS="$save_LIBS" case "$gl_cv_func_isnanf_works" in *yes) gl_func_isnanf=yes ;; *) gl_func_isnanf=no; ISNANF_LIBM= ;; esac else gl_func_isnanf=no fi if test $gl_func_isnanf != yes; then HAVE_ISNANF=0 fi AC_SUBST([ISNANF_LIBM]) ]) dnl Check how to get or define isnanf() without linking with libm. AC_DEFUN([gl_FUNC_ISNANF_NO_LIBM], [ gl_HAVE_ISNANF_NO_LIBM if test $gl_cv_func_isnanf_no_libm = yes; then gl_ISNANF_WORKS fi if test $gl_cv_func_isnanf_no_libm = yes \ && { case "$gl_cv_func_isnanf_works" in *yes) true;; *) false;; esac }; then gl_func_isnanf_no_libm=yes AC_DEFINE([HAVE_ISNANF_IN_LIBC], [1], [Define if the isnan(float) function is available in libc.]) else gl_func_isnanf_no_libm=no fi ]) dnl Prerequisites of replacement isnanf definition. It does not need -lm. AC_DEFUN([gl_PREREQ_ISNANF], [ gl_FLOAT_EXPONENT_LOCATION ]) dnl Test whether isnanf() can be used without libm. AC_DEFUN([gl_HAVE_ISNANF_NO_LIBM], [ AC_CACHE_CHECK([whether isnan(float) can be used without linking with libm], [gl_cv_func_isnanf_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #if __GNUC__ >= 4 # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) #elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) #endif float x;]], [[return isnanf (x);]])], [gl_cv_func_isnanf_no_libm=yes], [gl_cv_func_isnanf_no_libm=no]) ]) ]) dnl Test whether isnanf() can be used with libm. AC_DEFUN([gl_HAVE_ISNANF_IN_LIBM], [ AC_CACHE_CHECK([whether isnan(float) can be used with libm], [gl_cv_func_isnanf_in_libm], [ save_LIBS="$LIBS" LIBS="$LIBS -lm" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #if __GNUC__ >= 4 # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) #elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) #endif float x;]], [[return isnanf (x);]])], [gl_cv_func_isnanf_in_libm=yes], [gl_cv_func_isnanf_in_libm=no]) LIBS="$save_LIBS" ]) ]) dnl Test whether isnanf() rejects Infinity (this fails on Solaris 2.5.1), dnl recognizes a NaN (this fails on IRIX 6.5 with cc), and recognizes a NaN dnl with in-memory representation 0x7fbfffff (this fails on IRIX 6.5). AC_DEFUN([gl_ISNANF_WORKS], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_FLOAT_EXPONENT_LOCATION]) AC_CACHE_CHECK([whether isnan(float) works], [gl_cv_func_isnanf_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #if __GNUC__ >= 4 # undef isnanf # define isnanf(x) __builtin_isnanf ((float)(x)) #elif defined isnan # undef isnanf # define isnanf(x) isnan ((float)(x)) #endif /* The Compaq (ex-DEC) C 6.4 compiler chokes on the expression 0.0 / 0.0. */ #ifdef __DECC static float NaN () { static float zero = 0.0f; return zero / zero; } #else # define NaN() (0.0f / 0.0f) #endif #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { unsigned int word[NWORDS]; float value; } memory_float; int main() { int result = 0; if (isnanf (1.0f / 0.0f)) result |= 1; if (!isnanf (NaN ())) result |= 2; #if defined FLT_EXPBIT0_WORD && defined FLT_EXPBIT0_BIT /* The isnanf function should be immune against changes in the sign bit and in the mantissa bits. The xor operation twiddles a bit that can only be a sign bit or a mantissa bit. */ if (FLT_EXPBIT0_WORD == 0 && FLT_EXPBIT0_BIT > 0) { memory_float m; m.value = NaN (); /* Set the bits below the exponent to 01111...111. */ m.word[0] &= -1U << FLT_EXPBIT0_BIT; m.word[0] |= 1U << (FLT_EXPBIT0_BIT - 1) - 1; if (!isnanf (m.value)) result |= 4; } #endif return result; }]])], [gl_cv_func_isnanf_works=yes], [gl_cv_func_isnanf_works=no], [case "$host_os" in irix* | solaris*) gl_cv_func_isnanf_works="guessing no" ;; mingw*) # Guess yes on mingw, no on MSVC. AC_EGREP_CPP([Known], [ #ifdef __MINGW32__ Known #endif ], [gl_cv_func_isnanf_works="guessing yes"], [gl_cv_func_isnanf_works="guessing no"]) ;; *) gl_cv_func_isnanf_works="guessing yes" ;; esac ]) ]) ]) gnuastro-0.5/bootstrapped/m4/isnand.m40000644000175000017500000000525113217200022014675 00000000000000# isnand.m4 serial 11 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Check how to get or define isnand(). AC_DEFUN([gl_FUNC_ISNAND], [ AC_REQUIRE([gl_MATH_H_DEFAULTS]) ISNAND_LIBM= gl_HAVE_ISNAND_NO_LIBM if test $gl_cv_func_isnand_no_libm = no; then gl_HAVE_ISNAND_IN_LIBM if test $gl_cv_func_isnand_in_libm = yes; then ISNAND_LIBM=-lm fi fi dnl The variable gl_func_isnand set here is used by isnan.m4. if test $gl_cv_func_isnand_no_libm = yes \ || test $gl_cv_func_isnand_in_libm = yes; then gl_func_isnand=yes else gl_func_isnand=no HAVE_ISNAND=0 fi AC_SUBST([ISNAND_LIBM]) ]) dnl Check how to get or define isnand() without linking with libm. AC_DEFUN([gl_FUNC_ISNAND_NO_LIBM], [ gl_HAVE_ISNAND_NO_LIBM gl_func_isnand_no_libm=$gl_cv_func_isnand_no_libm if test $gl_cv_func_isnand_no_libm = yes; then AC_DEFINE([HAVE_ISNAND_IN_LIBC], [1], [Define if the isnan(double) function is available in libc.]) fi ]) dnl Prerequisites of replacement isnand definition. It does not need -lm. AC_DEFUN([gl_PREREQ_ISNAND], [ AC_REQUIRE([gl_DOUBLE_EXPONENT_LOCATION]) ]) dnl Test whether isnand() can be used with libm. AC_DEFUN([gl_HAVE_ISNAND_IN_LIBM], [ AC_CACHE_CHECK([whether isnan(double) can be used with libm], [gl_cv_func_isnand_in_libm], [ save_LIBS="$LIBS" LIBS="$LIBS -lm" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #if __GNUC__ >= 4 # undef isnand # define isnand(x) __builtin_isnan ((double)(x)) #elif defined isnan # undef isnand # define isnand(x) isnan ((double)(x)) #endif double x;]], [[return isnand (x);]])], [gl_cv_func_isnand_in_libm=yes], [gl_cv_func_isnand_in_libm=no]) LIBS="$save_LIBS" ]) ]) AC_DEFUN([gl_HAVE_ISNAND_NO_LIBM], [ AC_CACHE_CHECK([whether isnan(double) can be used without linking with libm], [gl_cv_func_isnand_no_libm], [ AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include #if __GNUC__ >= 4 # undef isnand # define isnand(x) __builtin_isnan ((double)(x)) #else # undef isnand # define isnand(x) isnan ((double)(x)) #endif double x;]], [[return isnand (x);]])], [gl_cv_func_isnand_no_libm=yes], [gl_cv_func_isnand_no_libm=no]) ]) ]) gnuastro-0.5/bootstrapped/m4/isblank.m40000644000175000017500000000103213217200022015035 00000000000000# isblank.m4 serial 3 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_ISBLANK], [ dnl Persuade glibc to declare isblank(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_CTYPE_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([isblank]) if test $ac_cv_func_isblank = no; then HAVE_ISBLANK=0 fi ]) gnuastro-0.5/bootstrapped/m4/ioctl.m40000644000175000017500000000305013217200022014526 00000000000000# ioctl.m4 serial 5 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_IOCTL], [ AC_REQUIRE([gl_SYS_IOCTL_H_DEFAULTS]) AC_REQUIRE([gl_HEADER_SYS_SOCKET]) HAVE_IOCTL=1 if test "$ac_cv_header_winsock2_h" = yes; then dnl Even if the 'socket' module is not used here, another part of the dnl application may use it and pass file descriptors that refer to dnl sockets to the ioctl() function. So enable the support for sockets. HAVE_IOCTL=0 else AC_CHECK_FUNCS([ioctl]) dnl On glibc systems, the second parameter is 'unsigned long int request', dnl not 'int request'. We cannot simply cast the function pointer, but dnl instead need a wrapper. AC_CACHE_CHECK([for ioctl with POSIX signature], [gl_cv_func_ioctl_posix_signature], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include /* On some platforms, ioctl() is declared in . */ #include ]], [[extern #ifdef __cplusplus "C" #endif int ioctl (int, int, ...); ]]) ], [gl_cv_func_ioctl_posix_signature=yes], [gl_cv_func_ioctl_posix_signature=no]) ]) if test $gl_cv_func_ioctl_posix_signature != yes; then REPLACE_IOCTL=1 fi fi ]) gnuastro-0.5/bootstrapped/m4/inttypes_h.m40000644000175000017500000000177413217200022015615 00000000000000# inttypes_h.m4 serial 10 dnl Copyright (C) 1997-2004, 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. # Define HAVE_INTTYPES_H_WITH_UINTMAX if exists, # doesn't clash with , and declares uintmax_t. AC_DEFUN([gl_AC_HEADER_INTTYPES_H], [ AC_CACHE_CHECK([for inttypes.h], [gl_cv_header_inttypes_h], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #include ]], [[uintmax_t i = (uintmax_t) -1; return !i;]])], [gl_cv_header_inttypes_h=yes], [gl_cv_header_inttypes_h=no])]) if test $gl_cv_header_inttypes_h = yes; then AC_DEFINE_UNQUOTED([HAVE_INTTYPES_H_WITH_UINTMAX], [1], [Define if exists, doesn't clash with , and declares uintmax_t. ]) fi ]) gnuastro-0.5/bootstrapped/m4/inttypes.m40000644000175000017500000001232013217200022015273 00000000000000# inttypes.m4 serial 26 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Derek Price, Bruno Haible. dnl Test whether is supported or must be substituted. AC_DEFUN([gl_INTTYPES_H], [ AC_REQUIRE([gl_INTTYPES_INCOMPLETE]) gl_INTTYPES_PRI_SCN ]) AC_DEFUN_ONCE([gl_INTTYPES_INCOMPLETE], [ AC_REQUIRE([gl_STDINT_H]) AC_CHECK_HEADERS_ONCE([inttypes.h]) dnl Override always, so that the portability warnings work. AC_REQUIRE([gl_INTTYPES_H_DEFAULTS]) gl_CHECK_NEXT_HEADERS([inttypes.h]) AC_REQUIRE([gl_MULTIARCH]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [imaxabs imaxdiv strtoimax strtoumax]) ]) # Ensure that the PRI* and SCN* macros are defined appropriately. AC_DEFUN([gl_INTTYPES_PRI_SCN], [ AC_REQUIRE([gt_INTTYPES_PRI]) PRIPTR_PREFIX= if test -n "$STDINT_H"; then dnl Using the gnulib . It always defines intptr_t to 'long'. PRIPTR_PREFIX='"l"' else dnl Using the system's . for glpfx in '' l ll I64; do case $glpfx in '') gltype1='int';; l) gltype1='long int';; ll) gltype1='long long int';; I64) gltype1='__int64';; esac AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[#include extern intptr_t foo; extern $gltype1 foo;]])], [PRIPTR_PREFIX='"'$glpfx'"']) test -n "$PRIPTR_PREFIX" && break done fi AC_SUBST([PRIPTR_PREFIX]) gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [INT32_MAX_LT_INTMAX_MAX], [defined INT32_MAX && defined INTMAX_MAX], [INT32_MAX < INTMAX_MAX], [sizeof (int) < sizeof (long long int)]) if test $APPLE_UNIVERSAL_BUILD = 0; then gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [INT64_MAX_EQ_LONG_MAX], [defined INT64_MAX], [INT64_MAX == LONG_MAX], [sizeof (long long int) == sizeof (long int)]) else INT64_MAX_EQ_LONG_MAX=-1 fi gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [UINT32_MAX_LT_UINTMAX_MAX], [defined UINT32_MAX && defined UINTMAX_MAX], [UINT32_MAX < UINTMAX_MAX], [sizeof (unsigned int) < sizeof (unsigned long long int)]) if test $APPLE_UNIVERSAL_BUILD = 0; then gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION( [UINT64_MAX_EQ_ULONG_MAX], [defined UINT64_MAX], [UINT64_MAX == ULONG_MAX], [sizeof (unsigned long long int) == sizeof (unsigned long int)]) else UINT64_MAX_EQ_ULONG_MAX=-1 fi ]) # Define the symbol $1 to be 1 if the condition is true, 0 otherwise. # If $2 is true, the condition is $3; otherwise if long long int is supported # approximate the condition with $4; otherwise, assume the condition is false. # The condition should work on all C99 platforms; the approximations should be # good enough to work on all practical pre-C99 platforms. # $2 is evaluated by the C preprocessor, $3 and $4 as compile-time constants. AC_DEFUN([gl_INTTYPES_CHECK_LONG_LONG_INT_CONDITION], [ AC_CACHE_CHECK([whether $3], [gl_cv_test_$1], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[/* Work also in C++ mode. */ #define __STDC_LIMIT_MACROS 1 /* Work if build is not clean. */ #define _GL_JUST_INCLUDE_SYSTEM_STDINT_H #include #if HAVE_STDINT_H #include #endif #if $2 #define CONDITION ($3) #elif HAVE_LONG_LONG_INT #define CONDITION ($4) #else #define CONDITION 0 #endif int test[CONDITION ? 1 : -1];]])], [gl_cv_test_$1=yes], [gl_cv_test_$1=no])]) if test $gl_cv_test_$1 = yes; then $1=1; else $1=0; fi AC_SUBST([$1]) ]) AC_DEFUN([gl_INTTYPES_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_INTTYPES_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_INTTYPES_H_DEFAULTS], [ GNULIB_IMAXABS=0; AC_SUBST([GNULIB_IMAXABS]) GNULIB_IMAXDIV=0; AC_SUBST([GNULIB_IMAXDIV]) GNULIB_STRTOIMAX=0; AC_SUBST([GNULIB_STRTOIMAX]) GNULIB_STRTOUMAX=0; AC_SUBST([GNULIB_STRTOUMAX]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_IMAXABS=1; AC_SUBST([HAVE_DECL_IMAXABS]) HAVE_DECL_IMAXDIV=1; AC_SUBST([HAVE_DECL_IMAXDIV]) HAVE_DECL_STRTOIMAX=1; AC_SUBST([HAVE_DECL_STRTOIMAX]) HAVE_DECL_STRTOUMAX=1; AC_SUBST([HAVE_DECL_STRTOUMAX]) REPLACE_STRTOIMAX=0; AC_SUBST([REPLACE_STRTOIMAX]) REPLACE_STRTOUMAX=0; AC_SUBST([REPLACE_STRTOUMAX]) INT32_MAX_LT_INTMAX_MAX=1; AC_SUBST([INT32_MAX_LT_INTMAX_MAX]) INT64_MAX_EQ_LONG_MAX='defined _LP64'; AC_SUBST([INT64_MAX_EQ_LONG_MAX]) PRI_MACROS_BROKEN=0; AC_SUBST([PRI_MACROS_BROKEN]) PRIPTR_PREFIX=__PRIPTR_PREFIX; AC_SUBST([PRIPTR_PREFIX]) UINT32_MAX_LT_UINTMAX_MAX=1; AC_SUBST([UINT32_MAX_LT_UINTMAX_MAX]) UINT64_MAX_EQ_ULONG_MAX='defined _LP64'; AC_SUBST([UINT64_MAX_EQ_ULONG_MAX]) ]) gnuastro-0.5/bootstrapped/m4/inttypes-pri.m40000644000175000017500000000234513217200022016071 00000000000000# inttypes-pri.m4 serial 7 (gettext-0.18.2) dnl Copyright (C) 1997-2002, 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_PREREQ([2.53]) # Define PRI_MACROS_BROKEN if exists and defines the PRI* # macros to non-string values. This is the case on AIX 4.3.3. AC_DEFUN([gt_INTTYPES_PRI], [ AC_CHECK_HEADERS([inttypes.h]) if test $ac_cv_header_inttypes_h = yes; then AC_CACHE_CHECK([whether the inttypes.h PRIxNN macros are broken], [gt_cv_inttypes_pri_broken], [ AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #ifdef PRId32 char *p = PRId32; #endif ]], [[]])], [gt_cv_inttypes_pri_broken=no], [gt_cv_inttypes_pri_broken=yes]) ]) fi if test "$gt_cv_inttypes_pri_broken" = yes; then AC_DEFINE_UNQUOTED([PRI_MACROS_BROKEN], [1], [Define if exists and defines unusable PRI* macros.]) PRI_MACROS_BROKEN=1 else PRI_MACROS_BROKEN=0 fi AC_SUBST([PRI_MACROS_BROKEN]) ]) gnuastro-0.5/bootstrapped/m4/intmax_t.m40000644000175000017500000000416613217200022015250 00000000000000# intmax_t.m4 serial 8 dnl Copyright (C) 1997-2004, 2006-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert. AC_PREREQ([2.53]) # Define intmax_t to 'long' or 'long long' # if it is not already defined in or . AC_DEFUN([gl_AC_TYPE_INTMAX_T], [ dnl For simplicity, we assume that a header file defines 'intmax_t' if and dnl only if it defines 'uintmax_t'. AC_REQUIRE([gl_AC_HEADER_INTTYPES_H]) AC_REQUIRE([gl_AC_HEADER_STDINT_H]) if test $gl_cv_header_inttypes_h = no && test $gl_cv_header_stdint_h = no; then AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) test $ac_cv_type_long_long_int = yes \ && ac_type='long long' \ || ac_type='long' AC_DEFINE_UNQUOTED([intmax_t], [$ac_type], [Define to long or long long if and don't define.]) else AC_DEFINE([HAVE_INTMAX_T], [1], [Define if you have the 'intmax_t' type in or .]) fi ]) dnl An alternative would be to explicitly test for 'intmax_t'. AC_DEFUN([gt_AC_TYPE_INTMAX_T], [ AC_REQUIRE([gl_AC_HEADER_INTTYPES_H]) AC_REQUIRE([gl_AC_HEADER_STDINT_H]) AC_CACHE_CHECK([for intmax_t], [gt_cv_c_intmax_t], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[ #include #include #if HAVE_STDINT_H_WITH_UINTMAX #include #endif #if HAVE_INTTYPES_H_WITH_UINTMAX #include #endif ]], [[intmax_t x = -1; return !x;]])], [gt_cv_c_intmax_t=yes], [gt_cv_c_intmax_t=no])]) if test $gt_cv_c_intmax_t = yes; then AC_DEFINE([HAVE_INTMAX_T], [1], [Define if you have the 'intmax_t' type in or .]) else AC_REQUIRE([AC_TYPE_LONG_LONG_INT]) test $ac_cv_type_long_long_int = yes \ && ac_type='long long' \ || ac_type='long' AC_DEFINE_UNQUOTED([intmax_t], [$ac_type], [Define to long or long long if and don't define.]) fi ]) gnuastro-0.5/bootstrapped/m4/intlmacosx.m40000644000175000017500000000474513217200022015611 00000000000000# intlmacosx.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2004-2014, 2016 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl dnl This file can be used in projects which are not available under dnl the GNU General Public License or the GNU Library General Public dnl License but which still want to provide support for the GNU gettext dnl functionality. dnl Please note that the actual code of the GNU gettext library is covered dnl by the GNU Library General Public License, and the rest of the GNU dnl gettext package is covered by the GNU General Public License. dnl They are *not* in the public domain. dnl Checks for special options needed on Mac OS X. dnl Defines INTL_MACOSX_LIBS. AC_DEFUN([gt_INTL_MACOSX], [ dnl Check for API introduced in Mac OS X 10.2. AC_CACHE_CHECK([for CFPreferencesCopyAppValue], [gt_cv_func_CFPreferencesCopyAppValue], [gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[CFPreferencesCopyAppValue(NULL, NULL)]])], [gt_cv_func_CFPreferencesCopyAppValue=yes], [gt_cv_func_CFPreferencesCopyAppValue=no]) LIBS="$gt_save_LIBS"]) if test $gt_cv_func_CFPreferencesCopyAppValue = yes; then AC_DEFINE([HAVE_CFPREFERENCESCOPYAPPVALUE], [1], [Define to 1 if you have the Mac OS X function CFPreferencesCopyAppValue in the CoreFoundation framework.]) fi dnl Check for API introduced in Mac OS X 10.3. AC_CACHE_CHECK([for CFLocaleCopyCurrent], [gt_cv_func_CFLocaleCopyCurrent], [gt_save_LIBS="$LIBS" LIBS="$LIBS -Wl,-framework -Wl,CoreFoundation" AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[CFLocaleCopyCurrent();]])], [gt_cv_func_CFLocaleCopyCurrent=yes], [gt_cv_func_CFLocaleCopyCurrent=no]) LIBS="$gt_save_LIBS"]) if test $gt_cv_func_CFLocaleCopyCurrent = yes; then AC_DEFINE([HAVE_CFLOCALECOPYCURRENT], [1], [Define to 1 if you have the Mac OS X function CFLocaleCopyCurrent in the CoreFoundation framework.]) fi INTL_MACOSX_LIBS= if test $gt_cv_func_CFPreferencesCopyAppValue = yes || test $gt_cv_func_CFLocaleCopyCurrent = yes; then INTL_MACOSX_LIBS="-Wl,-framework -Wl,CoreFoundation" fi AC_SUBST([INTL_MACOSX_LIBS]) ]) gnuastro-0.5/bootstrapped/m4/inet_pton.m40000644000175000017500000000422313217200022015416 00000000000000# inet_pton.m4 serial 18 dnl Copyright (C) 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_INET_PTON], [ AC_REQUIRE([gl_ARPA_INET_H_DEFAULTS]) dnl Persuade Solaris to declare inet_pton. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([AC_C_RESTRICT]) dnl Most platforms that provide inet_pton define it in libc. dnl Solaris 8..10 provide inet_pton in libnsl instead. dnl Solaris 2.6..7 provide inet_pton in libresolv instead. dnl Haiku provides it in -lnetwork. dnl Native Windows provides it in -lws2_32 instead, with a declaration in dnl , and it uses stdcall calling convention, not cdecl dnl (hence we cannot use AC_CHECK_FUNCS, AC_SEARCH_LIBS to find it). HAVE_INET_PTON=1 INET_PTON_LIB= gl_PREREQ_SYS_H_WINSOCK2 if test $HAVE_WINSOCK2_H = 1; then AC_CHECK_DECLS([inet_pton],,, [[#include ]]) if test $ac_cv_have_decl_inet_pton = yes; then dnl It needs to be overridden, because the stdcall calling convention dnl is not compliant with POSIX. REPLACE_INET_PTON=1 INET_PTON_LIB="-lws2_32" else HAVE_DECL_INET_PTON=0 HAVE_INET_PTON=0 fi else gl_save_LIBS=$LIBS AC_SEARCH_LIBS([inet_pton], [nsl resolv network], [], [AC_CHECK_FUNCS([inet_pton]) if test $ac_cv_func_inet_pton = no; then HAVE_INET_PTON=0 fi ]) LIBS=$gl_save_LIBS if test "$ac_cv_search_inet_pton" != "no" \ && test "$ac_cv_search_inet_pton" != "none required"; then INET_PTON_LIB="$ac_cv_search_inet_pton" fi AC_CHECK_HEADERS_ONCE([netdb.h]) AC_CHECK_DECLS([inet_pton],,, [[#include #if HAVE_NETDB_H # include #endif ]]) if test $ac_cv_have_decl_inet_pton = no; then HAVE_DECL_INET_PTON=0 fi fi AC_SUBST([INET_PTON_LIB]) ]) # Prerequisites of lib/inet_pton.c. AC_DEFUN([gl_PREREQ_INET_PTON], [ AC_REQUIRE([gl_SOCKET_FAMILIES]) ]) gnuastro-0.5/bootstrapped/m4/include_next.m40000644000175000017500000002106113217200022016077 00000000000000# include_next.m4 serial 24 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Paul Eggert and Derek Price. dnl Sets INCLUDE_NEXT, INCLUDE_NEXT_AS_FIRST_DIRECTIVE, PRAGMA_SYSTEM_HEADER, dnl and PRAGMA_COLUMNS. dnl dnl INCLUDE_NEXT expands to 'include_next' if the compiler supports it, or to dnl 'include' otherwise. dnl dnl INCLUDE_NEXT_AS_FIRST_DIRECTIVE expands to 'include_next' if the compiler dnl supports it in the special case that it is the first include directive in dnl the given file, or to 'include' otherwise. dnl dnl PRAGMA_SYSTEM_HEADER can be used in files that contain #include_next, dnl so as to avoid GCC warnings when the gcc option -pedantic is used. dnl '#pragma GCC system_header' has the same effect as if the file was found dnl through the include search path specified with '-isystem' options (as dnl opposed to the search path specified with '-I' options). Namely, gcc dnl does not warn about some things, and on some systems (Solaris and Interix) dnl __STDC__ evaluates to 0 instead of to 1. The latter is an undesired side dnl effect; we are therefore careful to use 'defined __STDC__' or '1' instead dnl of plain '__STDC__'. dnl dnl PRAGMA_COLUMNS can be used in files that override system header files, so dnl as to avoid compilation errors on HP NonStop systems when the gnulib file dnl is included by a system header file that does a "#pragma COLUMNS 80" (which dnl has the effect of truncating the lines of that file and all files that it dnl includes to 80 columns) and the gnulib file has lines longer than 80 dnl columns. AC_DEFUN([gl_INCLUDE_NEXT], [ AC_LANG_PREPROC_REQUIRE() AC_CACHE_CHECK([whether the preprocessor supports include_next], [gl_cv_have_include_next], [rm -rf conftestd1a conftestd1b conftestd2 mkdir conftestd1a conftestd1b conftestd2 dnl IBM C 9.0, 10.1 (original versions, prior to the 2009-01 updates) on dnl AIX 6.1 support include_next when used as first preprocessor directive dnl in a file, but not when preceded by another include directive. Check dnl for this bug by including . dnl Additionally, with this same compiler, include_next is a no-op when dnl used in a header file that was included by specifying its absolute dnl file name. Despite these two bugs, include_next is used in the dnl compiler's . By virtue of the second bug, we need to use dnl include_next as well in this case. cat < conftestd1a/conftest.h #define DEFINED_IN_CONFTESTD1 #include_next #ifdef DEFINED_IN_CONFTESTD2 int foo; #else #error "include_next doesn't work" #endif EOF cat < conftestd1b/conftest.h #define DEFINED_IN_CONFTESTD1 #include #include_next #ifdef DEFINED_IN_CONFTESTD2 int foo; #else #error "include_next doesn't work" #endif EOF cat < conftestd2/conftest.h #ifndef DEFINED_IN_CONFTESTD1 #error "include_next test doesn't work" #endif #define DEFINED_IN_CONFTESTD2 EOF gl_save_CPPFLAGS="$CPPFLAGS" CPPFLAGS="$gl_save_CPPFLAGS -Iconftestd1b -Iconftestd2" dnl We intentionally avoid using AC_LANG_SOURCE here. AC_COMPILE_IFELSE([AC_LANG_DEFINES_PROVIDED[#include ]], [gl_cv_have_include_next=yes], [CPPFLAGS="$gl_save_CPPFLAGS -Iconftestd1a -Iconftestd2" AC_COMPILE_IFELSE([AC_LANG_DEFINES_PROVIDED[#include ]], [gl_cv_have_include_next=buggy], [gl_cv_have_include_next=no]) ]) CPPFLAGS="$gl_save_CPPFLAGS" rm -rf conftestd1a conftestd1b conftestd2 ]) PRAGMA_SYSTEM_HEADER= if test $gl_cv_have_include_next = yes; then INCLUDE_NEXT=include_next INCLUDE_NEXT_AS_FIRST_DIRECTIVE=include_next if test -n "$GCC"; then PRAGMA_SYSTEM_HEADER='#pragma GCC system_header' fi else if test $gl_cv_have_include_next = buggy; then INCLUDE_NEXT=include INCLUDE_NEXT_AS_FIRST_DIRECTIVE=include_next else INCLUDE_NEXT=include INCLUDE_NEXT_AS_FIRST_DIRECTIVE=include fi fi AC_SUBST([INCLUDE_NEXT]) AC_SUBST([INCLUDE_NEXT_AS_FIRST_DIRECTIVE]) AC_SUBST([PRAGMA_SYSTEM_HEADER]) AC_CACHE_CHECK([whether system header files limit the line length], [gl_cv_pragma_columns], [dnl HP NonStop systems, which define __TANDEM, have this misfeature. AC_EGREP_CPP([choke me], [ #ifdef __TANDEM choke me #endif ], [gl_cv_pragma_columns=yes], [gl_cv_pragma_columns=no]) ]) if test $gl_cv_pragma_columns = yes; then PRAGMA_COLUMNS="#pragma COLUMNS 10000" else PRAGMA_COLUMNS= fi AC_SUBST([PRAGMA_COLUMNS]) ]) # gl_CHECK_NEXT_HEADERS(HEADER1 HEADER2 ...) # ------------------------------------------ # For each arg foo.h, if #include_next works, define NEXT_FOO_H to be # ''; otherwise define it to be # '"///usr/include/foo.h"', or whatever other absolute file name is suitable. # Also, if #include_next works as first preprocessing directive in a file, # define NEXT_AS_FIRST_DIRECTIVE_FOO_H to be ''; otherwise define it to # be # '"///usr/include/foo.h"', or whatever other absolute file name is suitable. # That way, a header file with the following line: # #@INCLUDE_NEXT@ @NEXT_FOO_H@ # or # #@INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ @NEXT_AS_FIRST_DIRECTIVE_FOO_H@ # behaves (after sed substitution) as if it contained # #include_next # even if the compiler does not support include_next. # The three "///" are to pacify Sun C 5.8, which otherwise would say # "warning: #include of /usr/include/... may be non-portable". # Use '""', not '<>', so that the /// cannot be confused with a C99 comment. # Note: This macro assumes that the header file is not empty after # preprocessing, i.e. it does not only define preprocessor macros but also # provides some type/enum definitions or function/variable declarations. # # This macro also checks whether each header exists, by invoking # AC_CHECK_HEADERS_ONCE or AC_CHECK_HEADERS on each argument. AC_DEFUN([gl_CHECK_NEXT_HEADERS], [ gl_NEXT_HEADERS_INTERNAL([$1], [check]) ]) # gl_NEXT_HEADERS(HEADER1 HEADER2 ...) # ------------------------------------ # Like gl_CHECK_NEXT_HEADERS, except do not check whether the headers exist. # This is suitable for headers like that are standardized by C89 # and therefore can be assumed to exist. AC_DEFUN([gl_NEXT_HEADERS], [ gl_NEXT_HEADERS_INTERNAL([$1], [assume]) ]) # The guts of gl_CHECK_NEXT_HEADERS and gl_NEXT_HEADERS. AC_DEFUN([gl_NEXT_HEADERS_INTERNAL], [ AC_REQUIRE([gl_INCLUDE_NEXT]) AC_REQUIRE([AC_CANONICAL_HOST]) m4_if([$2], [check], [AC_CHECK_HEADERS_ONCE([$1]) ]) dnl FIXME: gl_next_header and gl_header_exists must be used unquoted dnl until we can assume autoconf 2.64 or newer. m4_foreach_w([gl_HEADER_NAME], [$1], [AS_VAR_PUSHDEF([gl_next_header], [gl_cv_next_]m4_defn([gl_HEADER_NAME])) if test $gl_cv_have_include_next = yes; then AS_VAR_SET(gl_next_header, ['<'gl_HEADER_NAME'>']) else AC_CACHE_CHECK( [absolute name of <]m4_defn([gl_HEADER_NAME])[>], m4_defn([gl_next_header]), [m4_if([$2], [check], [AS_VAR_PUSHDEF([gl_header_exists], [ac_cv_header_]m4_defn([gl_HEADER_NAME])) if test AS_VAR_GET(gl_header_exists) = yes; then AS_VAR_POPDEF([gl_header_exists]) ]) gl_ABSOLUTE_HEADER_ONE(gl_HEADER_NAME) AS_VAR_COPY([gl_header], [gl_cv_absolute_]AS_TR_SH(gl_HEADER_NAME)) AS_VAR_SET(gl_next_header, ['"'$gl_header'"']) m4_if([$2], [check], [else AS_VAR_SET(gl_next_header, ['<'gl_HEADER_NAME'>']) fi ]) ]) fi AC_SUBST( AS_TR_CPP([NEXT_]m4_defn([gl_HEADER_NAME])), [AS_VAR_GET(gl_next_header)]) if test $gl_cv_have_include_next = yes || test $gl_cv_have_include_next = buggy; then # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include_next' gl_next_as_first_directive='<'gl_HEADER_NAME'>' else # INCLUDE_NEXT_AS_FIRST_DIRECTIVE='include' gl_next_as_first_directive=AS_VAR_GET(gl_next_header) fi AC_SUBST( AS_TR_CPP([NEXT_AS_FIRST_DIRECTIVE_]m4_defn([gl_HEADER_NAME])), [$gl_next_as_first_directive]) AS_VAR_POPDEF([gl_next_header])]) ]) # Autoconf 2.68 added warnings for our use of AC_COMPILE_IFELSE; # this fallback is safe for all earlier autoconf versions. m4_define_default([AC_LANG_DEFINES_PROVIDED]) gnuastro-0.5/bootstrapped/m4/host-cpu-c-abi.m40000644000175000017500000003043113217200022016132 00000000000000# host-cpu-c-abi.m4 serial 8 dnl Copyright (C) 2002-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible and Sam Steingold. dnl Sets the HOST_CPU variable to the canonical name of the CPU. dnl Sets the HOST_CPU_C_ABI variable to the canonical name of the CPU with its dnl C language ABI (application binary interface). dnl Also defines __${HOST_CPU}__ and __${HOST_CPU_C_ABI}__ as C macros in dnl config.h. dnl dnl This canonical name can be used to select a particular assembly language dnl source file that will interoperate with C code on the given host. dnl dnl For example: dnl * 'i386' and 'sparc' are different canonical names, because code for i386 dnl will not run on SPARC CPUs and vice versa. They have different dnl instruction sets. dnl * 'sparc' and 'sparc64' are different canonical names, because code for dnl 'sparc' and code for 'sparc64' cannot be linked together: 'sparc' code dnl contains 32-bit instructions, whereas 'sparc64' code contains 64-bit dnl instructions. A process on a SPARC CPU can be in 32-bit mode or in 64-bit dnl mode, but not both. dnl * 'mips' and 'mipsn32' are different canonical names, because they use dnl different argument passing and return conventions for C functions, and dnl although the instruction set of 'mips' is a large subset of the dnl instruction set of 'mipsn32'. dnl * 'mipsn32' and 'mips64' are different canonical names, because they use dnl different sizes for the C types like 'int' and 'void *', and although dnl the instruction sets of 'mipsn32' and 'mips64' are the same. dnl * The same canonical name is used for different endiannesses. You can dnl determine the endianness through preprocessor symbols: dnl - 'arm': test __ARMEL__. dnl - 'mips', 'mipsn32', 'mips64': test _MIPSEB vs. _MIPSEL. dnl - 'powerpc64': test _BIG_ENDIAN vs. _LITTLE_ENDIAN. dnl * The same name 'i386' is used for CPUs of type i386, i486, i586 dnl (Pentium), AMD K7, Pentium II, Pentium IV, etc., because dnl - Instructions that do not exist on all of these CPUs (cmpxchg, dnl MMX, SSE, SSE2, 3DNow! etc.) are not frequently used. If your dnl assembly language source files use such instructions, you will dnl need to make the distinction. dnl - Speed of execution of the common instruction set is reasonable across dnl the entire family of CPUs. If you have assembly language source files dnl that are optimized for particular CPU types (like GNU gmp has), you dnl will need to make the distinction. dnl See . AC_DEFUN([gl_HOST_CPU_C_ABI], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_C_ASM]) AC_CACHE_CHECK([host CPU and C ABI], [gl_cv_host_cpu_c_abi], [case "$host_cpu" in changequote(,)dnl i[4567]86 ) changequote([,])dnl gl_cv_host_cpu_c_abi=i386 ;; x86_64 ) # On x86_64 systems, the C compiler may be generating code in one of # these ABIs: # - 64-bit instruction set, 64-bit pointers, 64-bit 'long': x86_64. # - 64-bit instruction set, 64-bit pointers, 32-bit 'long': x86_64 # with native Windows (mingw, MSVC). # - 64-bit instruction set, 32-bit pointers, 32-bit 'long': x86_64-x32. # - 32-bit instruction set, 32-bit pointers, 32-bit 'long': i386. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if (defined __x86_64__ || defined __amd64__ \ || defined _M_X64 || defined _M_AMD64) int ok; #else error fail #endif ]])], [AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __ILP32__ || defined _ILP32 int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=x86_64-x32], [gl_cv_host_cpu_c_abi=x86_64])], [gl_cv_host_cpu_c_abi=i386]) ;; changequote(,)dnl alphaev[4-8] | alphaev56 | alphapca5[67] | alphaev6[78] ) changequote([,])dnl gl_cv_host_cpu_c_abi=alpha ;; arm* | aarch64 ) # Assume arm with EABI. # On arm64 systems, the C compiler may be generating code in one of # these ABIs: # - aarch64 instruction set, 64-bit pointers, 64-bit 'long': arm64. # - aarch64 instruction set, 32-bit pointers, 32-bit 'long': arm64-ilp32. # - 32-bit instruction set, 32-bit pointers, 32-bit 'long': arm or armhf. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#ifdef __aarch64__ int ok; #else error fail #endif ]])], [AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __ILP32__ || defined _ILP32 int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=arm64-ilp32], [gl_cv_host_cpu_c_abi=arm64])], [# Don't distinguish little-endian and big-endian arm, since they # don't require different machine code for simple operations and # since the user can distinguish them through the preprocessor # defines __ARMEL__ vs. __ARMEB__. # But distinguish arm which passes floating-point arguments and # return values in integer registers (r0, r1, ...) - this is # gcc -mfloat-abi=soft or gcc -mfloat-abi=softfp - from arm which # passes them in float registers (s0, s1, ...) and double registers # (d0, d1, ...) - this is gcc -mfloat-abi=hard. GCC 4.6 or newer # sets the preprocessor defines __ARM_PCS (for the first case) and # __ARM_PCS_VFP (for the second case), but older GCC does not. echo 'double ddd; void func (double dd) { ddd = dd; }' > conftest.c # Look for a reference to the register d0 in the .s file. AC_TRY_COMMAND(${CC-cc} $CFLAGS $CPPFLAGS $gl_c_asm_opt conftest.c) >/dev/null 2>&1 if LC_ALL=C grep -E 'd0,' conftest.$gl_asmext >/dev/null; then gl_cv_host_cpu_c_abi=armhf else gl_cv_host_cpu_c_abi=arm fi rm -f conftest* ]) ;; hppa1.0 | hppa1.1 | hppa2.0* | hppa64 ) # On hppa, the C compiler may be generating 32-bit code or 64-bit # code. In the latter case, it defines _LP64 and __LP64__. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#ifdef __LP64__ int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=hppa64], [gl_cv_host_cpu_c_abi=hppa]) ;; ia64* ) # On ia64 on HP-UX, the C compiler may be generating 64-bit code or # 32-bit code. In the latter case, it defines _ILP32. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#ifdef _ILP32 int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=ia64-ilp32], [gl_cv_host_cpu_c_abi=ia64]) ;; mips* ) # We should also check for (_MIPS_SZPTR == 64), but gcc keeps this # at 32. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined _MIPS_SZLONG && (_MIPS_SZLONG == 64) int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=mips64], [# In the n32 ABI, _ABIN32 is defined, _ABIO32 is not defined (but # may later get defined by ), and _MIPS_SIM == _ABIN32. # In the 32 ABI, _ABIO32 is defined, _ABIN32 is not defined (but # may later get defined by ), and _MIPS_SIM == _ABIO32. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if (_MIPS_SIM == _ABIN32) int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=mipsn32], [gl_cv_host_cpu_c_abi=mips])]) ;; powerpc* ) # Different ABIs are in use on AIX vs. Mac OS X vs. Linux,*BSD. # No need to distinguish them here; the caller may distinguish # them based on the OS. # On powerpc64 systems, the C compiler may still be generating # 32-bit code. And on powerpc-ibm-aix systems, the C compiler may # be generating 64-bit code. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __powerpc64__ || defined _ARCH_PPC64 int ok; #else error fail #endif ]])], [# On powerpc64, there are two ABIs on Linux: The AIX compatible # one and the ELFv2 one. The latter defines _CALL_ELF=2. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined _CALL_ELF && _CALL_ELF == 2 int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=powerpc64-elfv2], [gl_cv_host_cpu_c_abi=powerpc64]) ], [gl_cv_host_cpu_c_abi=powerpc]) ;; rs6000 ) gl_cv_host_cpu_c_abi=powerpc ;; s390* ) # On s390x, the C compiler may be generating 64-bit (= s390x) code # or 31-bit (= s390) code. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __LP64__ || defined __s390x__ int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=s390x], [gl_cv_host_cpu_c_abi=s390]) ;; sparc | sparc64 ) # UltraSPARCs running Linux have `uname -m` = "sparc64", but the # C compiler still generates 32-bit code. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __sparcv9 || defined __arch64__ int ok; #else error fail #endif ]])], [gl_cv_host_cpu_c_abi=sparc64], [gl_cv_host_cpu_c_abi=sparc]) ;; *) gl_cv_host_cpu_c_abi="$host_cpu" ;; esac ]) dnl In most cases, $HOST_CPU and $HOST_CPU_C_ABI are the same. HOST_CPU=`echo "$gl_cv_host_cpu_c_abi" | sed -e 's/-.*//'` HOST_CPU_C_ABI="$gl_cv_host_cpu_c_abi" AC_SUBST([HOST_CPU]) AC_SUBST([HOST_CPU_C_ABI]) # This was # AC_DEFINE_UNQUOTED([__${HOST_CPU}__]) # AC_DEFINE_UNQUOTED([__${HOST_CPU_C_ABI}__]) # earlier, but KAI C++ 3.2d doesn't like this. sed -e 's/-/_/g' >> confdefs.h <. # # As a special exception to the GNU General Public License, # this file may be distributed as part of a program that # contains a configuration script generated by Autoconf, under # the same distribution terms as the rest of that program. # # Generated by gnulib-tool. # # This file represents the compiled summary of the specification in # gnulib-cache.m4. It lists the computed macro invocations that need # to be invoked from configure.ac. # In projects that use version control, this file can be treated like # other built files. # This macro should be invoked from ./configure.ac, in the section # "Checks for programs", right after AC_PROG_CC, and certainly before # any checks for libraries, header files, types and library functions. AC_DEFUN([gl_EARLY], [ m4_pattern_forbid([^gl_[A-Z]])dnl the gnulib macro namespace m4_pattern_allow([^gl_ES$])dnl a valid locale name m4_pattern_allow([^gl_LIBOBJS$])dnl a variable m4_pattern_allow([^gl_LTLIBOBJS$])dnl a variable # Pre-early section. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_PROG_AR_RANLIB]) AC_REQUIRE([AM_PROG_CC_C_O]) # Code from module absolute-header: # Code from module accept: # Code from module accept-tests: # Code from module alloca: # Code from module alloca-opt: # Code from module alloca-opt-tests: # Code from module argp: # Code from module argp-tests: # Code from module arpa_inet: # Code from module arpa_inet-tests: # Code from module binary-io: # Code from module binary-io-tests: # Code from module bind: # Code from module bind-tests: # Code from module btowc: # Code from module btowc-tests: # Code from module builtin-expect: # Code from module c-ctype: # Code from module c-ctype-tests: # Code from module c-strcase: # Code from module c-strcase-tests: # Code from module cloexec: # Code from module cloexec-tests: # Code from module close: # Code from module close-tests: # Code from module configmake: # Code from module connect: # Code from module connect-tests: # Code from module ctype: # Code from module ctype-tests: # Code from module dirname-lgpl: # Code from module dosname: # Code from module double-slash-root: # Code from module dup2: # Code from module dup2-tests: # Code from module environ: # Code from module environ-tests: # Code from module errno: # Code from module errno-tests: # Code from module error: # Code from module extensions: # Code from module extern-inline: # Code from module fcntl: # Code from module fcntl-h: # Code from module fcntl-h-tests: # Code from module fcntl-tests: # Code from module fd-hook: # Code from module fdl: # Code from module fdopen: # Code from module fdopen-tests: # Code from module fgetc-tests: # Code from module filename: # Code from module flexmember: # Code from module float: # Code from module float-tests: # Code from module fpieee: AC_REQUIRE([gl_FP_IEEE]) # Code from module fpucw: # Code from module fputc-tests: # Code from module fread-tests: # Code from module fstat: # Code from module fstat-tests: # Code from module ftruncate: # Code from module ftruncate-tests: # Code from module func: # Code from module func-tests: # Code from module fwrite-tests: # Code from module gendocs: # Code from module getcwd-lgpl: # Code from module getcwd-lgpl-tests: # Code from module getdelim: # Code from module getdelim-tests: # Code from module getdtablesize: # Code from module getdtablesize-tests: # Code from module getline: # Code from module getline-tests: # Code from module getopt-gnu: # Code from module getopt-gnu-tests: # Code from module getopt-posix: # Code from module getopt-posix-tests: # Code from module getpagesize: # Code from module getprogname: # Code from module getprogname-tests: # Code from module gettext-h: # Code from module gettimeofday: # Code from module gettimeofday-tests: # Code from module git-version-gen: # Code from module hard-locale: # Code from module havelib: # Code from module host-cpu-c-abi: # Code from module ignore-value: # Code from module ignore-value-tests: # Code from module include_next: # Code from module inet_pton: # Code from module inet_pton-tests: # Code from module intprops: # Code from module intprops-tests: # Code from module inttypes: # Code from module inttypes-incomplete: # Code from module inttypes-tests: # Code from module ioctl: # Code from module ioctl-tests: # Code from module isblank: # Code from module isblank-tests: # Code from module isnand-nolibm: # Code from module isnand-nolibm-tests: # Code from module isnanf-nolibm: # Code from module isnanf-nolibm-tests: # Code from module isnanl-nolibm: # Code from module isnanl-nolibm-tests: # Code from module iswblank: # Code from module iswblank-tests: # Code from module langinfo: # Code from module langinfo-tests: # Code from module largefile: AC_REQUIRE([AC_SYS_LARGEFILE]) # Code from module limits-h: # Code from module limits-h-tests: # Code from module listen: # Code from module listen-tests: # Code from module localcharset: # Code from module locale: # Code from module locale-tests: # Code from module localeconv: # Code from module localeconv-tests: # Code from module localename: # Code from module localename-tests: # Code from module localtime-buffer: # Code from module lock: # Code from module lock-tests: # Code from module lstat: # Code from module lstat-tests: # Code from module malloc-gnu: # Code from module malloc-gnu-tests: # Code from module malloc-posix: # Code from module malloca: # Code from module malloca-tests: # Code from module math: # Code from module math-tests: # Code from module mbchar: # Code from module mbrtowc: # Code from module mbrtowc-tests: # Code from module mbschr: # Code from module mbschr-tests: # Code from module mbsinit: # Code from module mbsinit-tests: # Code from module mbspbrk: # Code from module mbspbrk-tests: # Code from module mbsspn: # Code from module mbsspn-tests: # Code from module mbstok_r: # Code from module mbtowc: # Code from module mbuiter: # Code from module memchr: # Code from module memchr-tests: # Code from module mempcpy: # Code from module minmax: # Code from module msvc-inval: # Code from module msvc-nothrow: # Code from module multiarch: # Code from module nanosleep: # Code from module nanosleep-tests: # Code from module netinet_in: # Code from module netinet_in-tests: # Code from module nl_langinfo: # Code from module nl_langinfo-tests: # Code from module nocrash: # Code from module nproc: # Code from module open: # Code from module open-tests: # Code from module pathmax: # Code from module pathmax-tests: # Code from module perror: # Code from module perror-tests: # Code from module pipe-posix: # Code from module pipe-posix-tests: # Code from module pthread_sigmask: # Code from module pthread_sigmask-tests: # Code from module putenv: # Code from module raise: # Code from module raise-tests: # Code from module rawmemchr: # Code from module rawmemchr-tests: # Code from module regex: # Code from module regex-tests: # Code from module same-inode: # Code from module select: # Code from module select-tests: # Code from module setenv: # Code from module setenv-tests: # Code from module setlocale: # Code from module setlocale-tests: # Code from module setsockopt: # Code from module setsockopt-tests: # Code from module sigaction: # Code from module sigaction-tests: # Code from module signal-h: # Code from module signal-h-tests: # Code from module signbit: # Code from module signbit-tests: # Code from module sigprocmask: # Code from module sigprocmask-tests: # Code from module size_max: # Code from module sleep: # Code from module sleep-tests: # Code from module snippet/_Noreturn: # Code from module snippet/arg-nonnull: # Code from module snippet/c++defs: # Code from module snippet/warn-on-use: # Code from module socket: # Code from module socketlib: # Code from module sockets: # Code from module sockets-tests: # Code from module socklen: # Code from module ssize_t: # Code from module stat: # Code from module stat-tests: # Code from module stat-time: # Code from module stat-time-tests: # Code from module stdalign: # Code from module stdalign-tests: # Code from module stdbool: # Code from module stdbool-tests: # Code from module stddef: # Code from module stddef-tests: # Code from module stdint: # Code from module stdint-tests: # Code from module stdio: # Code from module stdio-tests: # Code from module stdlib: # Code from module stdlib-tests: # Code from module strcase: # Code from module strchrnul: # Code from module strchrnul-tests: # Code from module streq: # Code from module strerror: # Code from module strerror-override: # Code from module strerror-tests: # Code from module strerror_r-posix: # Code from module strerror_r-posix-tests: # Code from module string: # Code from module string-tests: # Code from module strings: # Code from module strings-tests: # Code from module strndup: # Code from module strnlen: # Code from module strnlen-tests: # Code from module strnlen1: # Code from module strtod: # Code from module strtod-tests: # Code from module strtok_r: # Code from module symlink: # Code from module symlink-tests: # Code from module sys_ioctl: # Code from module sys_ioctl-tests: # Code from module sys_select: # Code from module sys_select-tests: # Code from module sys_socket: # Code from module sys_socket-tests: # Code from module sys_stat: # Code from module sys_stat-tests: # Code from module sys_time: # Code from module sys_time-tests: # Code from module sys_types: # Code from module sys_types-tests: # Code from module sys_uio: # Code from module sys_uio-tests: # Code from module sysexits: # Code from module sysexits-tests: # Code from module test-framework-sh: # Code from module test-framework-sh-tests: # Code from module thread: # Code from module thread-tests: # Code from module threadlib: gl_THREADLIB_EARLY # Code from module time: # Code from module time-tests: # Code from module unistd: # Code from module unistd-tests: # Code from module unitypes: # Code from module uniwidth/base: # Code from module uniwidth/width: # Code from module uniwidth/width-tests: # Code from module unsetenv: # Code from module unsetenv-tests: # Code from module usleep: # Code from module usleep-tests: # Code from module vasnprintf: # Code from module vasnprintf-tests: # Code from module verify: # Code from module verify-tests: # Code from module vsnprintf: # Code from module vsnprintf-tests: # Code from module wchar: # Code from module wchar-tests: # Code from module wcrtomb: # Code from module wcrtomb-tests: # Code from module wctob: # Code from module wctomb: # Code from module wctype-h: # Code from module wctype-h-tests: # Code from module wcwidth: # Code from module wcwidth-tests: # Code from module xalloc-oversized: # Code from module xsize: # Code from module yield: ]) # This macro should be invoked from ./configure.ac, in the section # "Check for header files, types and library functions". AC_DEFUN([gl_INIT], [ AM_CONDITIONAL([GL_COND_LIBTOOL], [true]) gl_cond_libtool=true gl_m4_base='bootstrapped/m4' m4_pushdef([AC_LIBOBJ], m4_defn([gl_LIBOBJ])) m4_pushdef([AC_REPLACE_FUNCS], m4_defn([gl_REPLACE_FUNCS])) m4_pushdef([AC_LIBSOURCES], m4_defn([gl_LIBSOURCES])) m4_pushdef([gl_LIBSOURCES_LIST], []) m4_pushdef([gl_LIBSOURCES_DIR], []) gl_COMMON gl_source_base='bootstrapped/lib' changequote(,)dnl LTALLOCA=`echo "$ALLOCA" | sed -e 's/\.[^.]* /.lo /g;s/\.[^.]*$/.lo/'` changequote([, ])dnl AC_SUBST([LTALLOCA]) gl_FUNC_ALLOCA gl_ARGP m4_ifdef([AM_XGETTEXT_OPTION], [AM_][XGETTEXT_OPTION([--flag=argp_error:2:c-format]) AM_][XGETTEXT_OPTION([--flag=argp_failure:4:c-format])]) gl_FUNC_BTOWC if test $HAVE_BTOWC = 0 || test $REPLACE_BTOWC = 1; then AC_LIBOBJ([btowc]) gl_PREREQ_BTOWC fi gl_WCHAR_MODULE_INDICATOR([btowc]) gl___BUILTIN_EXPECT gl_CONFIGMAKE_PREP gl_DIRNAME_LGPL gl_DOUBLE_SLASH_ROOT gl_HEADER_ERRNO_H gl_ERROR if test $ac_cv_lib_error_at_line = no; then AC_LIBOBJ([error]) gl_PREREQ_ERROR fi m4_ifdef([AM_XGETTEXT_OPTION], [AM_][XGETTEXT_OPTION([--flag=error:3:c-format]) AM_][XGETTEXT_OPTION([--flag=error_at_line:5:c-format])]) AC_REQUIRE([gl_EXTERN_INLINE]) gl_FLOAT_H if test $REPLACE_FLOAT_LDBL = 1; then AC_LIBOBJ([float]) fi if test $REPLACE_ITOLD = 1; then AC_LIBOBJ([itold]) fi gl_FUNC gl_FUNC_GETDELIM if test $HAVE_GETDELIM = 0 || test $REPLACE_GETDELIM = 1; then AC_LIBOBJ([getdelim]) gl_PREREQ_GETDELIM fi gl_STDIO_MODULE_INDICATOR([getdelim]) gl_FUNC_GETLINE if test $REPLACE_GETLINE = 1; then AC_LIBOBJ([getline]) gl_PREREQ_GETLINE fi gl_STDIO_MODULE_INDICATOR([getline]) gl_FUNC_GETOPT_GNU dnl Because of the way gl_FUNC_GETOPT_GNU is implemented (the gl_getopt_required dnl mechanism), there is no need to do any AC_LIBOBJ or AC_SUBST here; they are dnl done in the getopt-posix module. gl_FUNC_GETOPT_POSIX if test $REPLACE_GETOPT = 1; then AC_LIBOBJ([getopt]) AC_LIBOBJ([getopt1]) dnl Arrange for unistd.h to include getopt.h. GNULIB_GL_UNISTD_H_GETOPT=1 fi AC_SUBST([GNULIB_GL_UNISTD_H_GETOPT]) gl_FUNC_GETPROGNAME AC_SUBST([LIBINTL]) AC_SUBST([LTLIBINTL]) gl_HARD_LOCALE AC_REQUIRE([gl_HOST_CPU_C_ABI]) gl_INTTYPES_H gl_INTTYPES_INCOMPLETE gl_FUNC_ISWBLANK if test $HAVE_ISWCNTRL = 0 || test $REPLACE_ISWCNTRL = 1; then : else if test $HAVE_ISWBLANK = 0 || test $REPLACE_ISWBLANK = 1; then AC_LIBOBJ([iswblank]) fi fi gl_WCTYPE_MODULE_INDICATOR([iswblank]) gl_LANGINFO_H gl_LIMITS_H gl_LOCALCHARSET LOCALCHARSET_TESTS_ENVIRONMENT="CHARSETALIASDIR=\"\$(abs_top_builddir)/$gl_source_base\"" AC_SUBST([LOCALCHARSET_TESTS_ENVIRONMENT]) gl_LOCALE_H gl_FUNC_LOCALECONV if test $REPLACE_LOCALECONV = 1; then AC_LIBOBJ([localeconv]) gl_PREREQ_LOCALECONV fi gl_LOCALE_MODULE_INDICATOR([localeconv]) gl_LOCK gl_MODULE_INDICATOR([lock]) gl_FUNC_MALLOC_GNU if test $REPLACE_MALLOC = 1; then AC_LIBOBJ([malloc]) fi gl_MODULE_INDICATOR([malloc-gnu]) gl_FUNC_MALLOC_POSIX if test $REPLACE_MALLOC = 1; then AC_LIBOBJ([malloc]) fi gl_STDLIB_MODULE_INDICATOR([malloc-posix]) gl_MATH_H gl_MBCHAR gl_FUNC_MBRTOWC if test $HAVE_MBRTOWC = 0 || test $REPLACE_MBRTOWC = 1; then AC_LIBOBJ([mbrtowc]) gl_PREREQ_MBRTOWC fi gl_WCHAR_MODULE_INDICATOR([mbrtowc]) gl_STRING_MODULE_INDICATOR([mbschr]) gl_FUNC_MBSINIT if test $HAVE_MBSINIT = 0 || test $REPLACE_MBSINIT = 1; then AC_LIBOBJ([mbsinit]) gl_PREREQ_MBSINIT fi gl_WCHAR_MODULE_INDICATOR([mbsinit]) gl_STRING_MODULE_INDICATOR([mbspbrk]) gl_STRING_MODULE_INDICATOR([mbsspn]) gl_STRING_MODULE_INDICATOR([mbstok_r]) gl_FUNC_MBTOWC if test $REPLACE_MBTOWC = 1; then AC_LIBOBJ([mbtowc]) gl_PREREQ_MBTOWC fi gl_STDLIB_MODULE_INDICATOR([mbtowc]) gl_MBITER gl_FUNC_MEMCHR if test $HAVE_MEMCHR = 0 || test $REPLACE_MEMCHR = 1; then AC_LIBOBJ([memchr]) gl_PREREQ_MEMCHR fi gl_STRING_MODULE_INDICATOR([memchr]) gl_FUNC_MEMPCPY if test $HAVE_MEMPCPY = 0; then AC_LIBOBJ([mempcpy]) gl_PREREQ_MEMPCPY fi gl_STRING_MODULE_INDICATOR([mempcpy]) gl_MINMAX AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then AC_LIBOBJ([msvc-inval]) fi AC_REQUIRE([gl_MSVC_NOTHROW]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then AC_LIBOBJ([msvc-nothrow]) fi gl_MODULE_INDICATOR([msvc-nothrow]) gl_MULTIARCH gl_FUNC_NL_LANGINFO if test $HAVE_NL_LANGINFO = 0 || test $REPLACE_NL_LANGINFO = 1; then AC_LIBOBJ([nl_langinfo]) fi gl_LANGINFO_MODULE_INDICATOR([nl_langinfo]) gl_NPROC gl_FUNC_RAWMEMCHR if test $HAVE_RAWMEMCHR = 0; then AC_LIBOBJ([rawmemchr]) gl_PREREQ_RAWMEMCHR fi gl_STRING_MODULE_INDICATOR([rawmemchr]) gl_REGEX if test $ac_use_included_regex = yes; then AC_LIBOBJ([regex]) gl_PREREQ_REGEX fi gl_SIZE_MAX gl_FUNC_SLEEP if test $HAVE_SLEEP = 0 || test $REPLACE_SLEEP = 1; then AC_LIBOBJ([sleep]) fi gl_UNISTD_MODULE_INDICATOR([sleep]) gt_TYPE_SSIZE_T gl_STDALIGN_H AM_STDBOOL_H gl_STDDEF_H gl_STDINT_H gl_STDIO_H gl_STDLIB_H gl_STRCASE if test $HAVE_STRCASECMP = 0; then AC_LIBOBJ([strcasecmp]) gl_PREREQ_STRCASECMP fi if test $HAVE_STRNCASECMP = 0; then AC_LIBOBJ([strncasecmp]) gl_PREREQ_STRNCASECMP fi gl_FUNC_STRCHRNUL if test $HAVE_STRCHRNUL = 0 || test $REPLACE_STRCHRNUL = 1; then AC_LIBOBJ([strchrnul]) gl_PREREQ_STRCHRNUL fi gl_STRING_MODULE_INDICATOR([strchrnul]) gl_FUNC_STRERROR if test $REPLACE_STRERROR = 1; then AC_LIBOBJ([strerror]) fi gl_MODULE_INDICATOR([strerror]) gl_STRING_MODULE_INDICATOR([strerror]) AC_REQUIRE([gl_HEADER_ERRNO_H]) AC_REQUIRE([gl_FUNC_STRERROR_0]) if test -n "$ERRNO_H" || test $REPLACE_STRERROR_0 = 1; then AC_LIBOBJ([strerror-override]) gl_PREREQ_SYS_H_WINSOCK2 fi gl_HEADER_STRING_H gl_HEADER_STRINGS_H gl_FUNC_STRNDUP if test $HAVE_STRNDUP = 0 || test $REPLACE_STRNDUP = 1; then AC_LIBOBJ([strndup]) fi gl_STRING_MODULE_INDICATOR([strndup]) gl_FUNC_STRNLEN if test $HAVE_DECL_STRNLEN = 0 || test $REPLACE_STRNLEN = 1; then AC_LIBOBJ([strnlen]) gl_PREREQ_STRNLEN fi gl_STRING_MODULE_INDICATOR([strnlen]) gl_FUNC_STRTOD if test $HAVE_STRTOD = 0 || test $REPLACE_STRTOD = 1; then AC_LIBOBJ([strtod]) gl_PREREQ_STRTOD fi gl_STDLIB_MODULE_INDICATOR([strtod]) gl_FUNC_STRTOK_R if test $HAVE_STRTOK_R = 0 || test $REPLACE_STRTOK_R = 1; then AC_LIBOBJ([strtok_r]) gl_PREREQ_STRTOK_R fi gl_STRING_MODULE_INDICATOR([strtok_r]) gl_SYS_TYPES_H AC_PROG_MKDIR_P gl_SYSEXITS gl_THREADLIB gl_UNISTD_H gl_LIBUNISTRING_LIBHEADER([0.9.4], [unitypes.h]) gl_LIBUNISTRING_LIBHEADER([0.9.4], [uniwidth.h]) gl_LIBUNISTRING_MODULE([0.9.8], [uniwidth/width]) gl_FUNC_VASNPRINTF gl_FUNC_VSNPRINTF gl_STDIO_MODULE_INDICATOR([vsnprintf]) gl_WCHAR_H gl_FUNC_WCRTOMB if test $HAVE_WCRTOMB = 0 || test $REPLACE_WCRTOMB = 1; then AC_LIBOBJ([wcrtomb]) gl_PREREQ_WCRTOMB fi gl_WCHAR_MODULE_INDICATOR([wcrtomb]) gl_WCTYPE_H gl_FUNC_WCWIDTH if test $HAVE_WCWIDTH = 0 || test $REPLACE_WCWIDTH = 1; then AC_LIBOBJ([wcwidth]) fi gl_WCHAR_MODULE_INDICATOR([wcwidth]) gl_XSIZE # End of code from modules m4_ifval(gl_LIBSOURCES_LIST, [ m4_syscmd([test ! -d ]m4_defn([gl_LIBSOURCES_DIR])[ || for gl_file in ]gl_LIBSOURCES_LIST[ ; do if test ! -r ]m4_defn([gl_LIBSOURCES_DIR])[/$gl_file ; then echo "missing file ]m4_defn([gl_LIBSOURCES_DIR])[/$gl_file" >&2 exit 1 fi done])dnl m4_if(m4_sysval, [0], [], [AC_FATAL([expected source file, required through AC_LIBSOURCES, not found])]) ]) m4_popdef([gl_LIBSOURCES_DIR]) m4_popdef([gl_LIBSOURCES_LIST]) m4_popdef([AC_LIBSOURCES]) m4_popdef([AC_REPLACE_FUNCS]) m4_popdef([AC_LIBOBJ]) AC_CONFIG_COMMANDS_PRE([ gl_libobjs= gl_ltlibobjs= if test -n "$gl_LIBOBJS"; then # Remove the extension. sed_drop_objext='s/\.o$//;s/\.obj$//' for i in `for i in $gl_LIBOBJS; do echo "$i"; done | sed -e "$sed_drop_objext" | sort | uniq`; do gl_libobjs="$gl_libobjs $i.$ac_objext" gl_ltlibobjs="$gl_ltlibobjs $i.lo" done fi AC_SUBST([gl_LIBOBJS], [$gl_libobjs]) AC_SUBST([gl_LTLIBOBJS], [$gl_ltlibobjs]) ]) gltests_libdeps= gltests_ltlibdeps= m4_pushdef([AC_LIBOBJ], m4_defn([gltests_LIBOBJ])) m4_pushdef([AC_REPLACE_FUNCS], m4_defn([gltests_REPLACE_FUNCS])) m4_pushdef([AC_LIBSOURCES], m4_defn([gltests_LIBSOURCES])) m4_pushdef([gltests_LIBSOURCES_LIST], []) m4_pushdef([gltests_LIBSOURCES_DIR], []) gl_COMMON gl_source_base='bootstrapped/tests' changequote(,)dnl gltests_WITNESS=IN_`echo "${PACKAGE-$PACKAGE_TARNAME}" | LC_ALL=C tr abcdefghijklmnopqrstuvwxyz ABCDEFGHIJKLMNOPQRSTUVWXYZ | LC_ALL=C sed -e 's/[^A-Z0-9_]/_/g'`_GNULIB_TESTS changequote([, ])dnl AC_SUBST([gltests_WITNESS]) gl_module_indicator_condition=$gltests_WITNESS m4_pushdef([gl_MODULE_INDICATOR_CONDITION], [$gl_module_indicator_condition]) AC_REQUIRE([gl_HEADER_SYS_SOCKET]) if test "$ac_cv_header_winsock2_h" = yes; then AC_LIBOBJ([accept]) fi gl_SYS_SOCKET_MODULE_INDICATOR([accept]) gl_HEADER_ARPA_INET AC_PROG_MKDIR_P AC_REQUIRE([gl_HEADER_SYS_SOCKET]) if test "$ac_cv_header_winsock2_h" = yes; then AC_LIBOBJ([bind]) fi gl_SYS_SOCKET_MODULE_INDICATOR([bind]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_FR gt_LOCALE_TR_UTF8 gl_MODULE_INDICATOR_FOR_TESTS([cloexec]) gl_FUNC_CLOSE if test $REPLACE_CLOSE = 1; then AC_LIBOBJ([close]) fi gl_UNISTD_MODULE_INDICATOR([close]) AC_REQUIRE([gl_HEADER_SYS_SOCKET]) if test "$ac_cv_header_winsock2_h" = yes; then AC_LIBOBJ([connect]) fi gl_SYS_SOCKET_MODULE_INDICATOR([connect]) gl_CTYPE_H gl_FUNC_DUP2 if test $HAVE_DUP2 = 0 || test $REPLACE_DUP2 = 1; then AC_LIBOBJ([dup2]) gl_PREREQ_DUP2 fi gl_UNISTD_MODULE_INDICATOR([dup2]) gl_ENVIRON gl_UNISTD_MODULE_INDICATOR([environ]) gl_FUNC_FCNTL if test $HAVE_FCNTL = 0 || test $REPLACE_FCNTL = 1; then AC_LIBOBJ([fcntl]) fi gl_FCNTL_MODULE_INDICATOR([fcntl]) gl_FCNTL_H gl_FUNC_FDOPEN if test $REPLACE_FDOPEN = 1; then AC_LIBOBJ([fdopen]) gl_PREREQ_FDOPEN fi gl_STDIO_MODULE_INDICATOR([fdopen]) AC_C_FLEXIBLE_ARRAY_MEMBER gl_FUNC_FSTAT if test $REPLACE_FSTAT = 1; then AC_LIBOBJ([fstat]) case "$host_os" in mingw*) AC_LIBOBJ([stat-w32]) ;; esac gl_PREREQ_FSTAT fi gl_SYS_STAT_MODULE_INDICATOR([fstat]) gl_FUNC_FTRUNCATE if test $HAVE_FTRUNCATE = 0 || test $REPLACE_FTRUNCATE = 1; then AC_LIBOBJ([ftruncate]) gl_PREREQ_FTRUNCATE fi gl_UNISTD_MODULE_INDICATOR([ftruncate]) gl_FUNC_GETCWD_LGPL if test $REPLACE_GETCWD = 1; then AC_LIBOBJ([getcwd-lgpl]) fi gl_UNISTD_MODULE_INDICATOR([getcwd]) gl_FUNC_GETDTABLESIZE if test $HAVE_GETDTABLESIZE = 0 || test $REPLACE_GETDTABLESIZE = 1; then AC_LIBOBJ([getdtablesize]) gl_PREREQ_GETDTABLESIZE fi gl_UNISTD_MODULE_INDICATOR([getdtablesize]) gl_FUNC_GETPAGESIZE if test $REPLACE_GETPAGESIZE = 1; then AC_LIBOBJ([getpagesize]) fi gl_UNISTD_MODULE_INDICATOR([getpagesize]) gl_FUNC_GETTIMEOFDAY if test $HAVE_GETTIMEOFDAY = 0 || test $REPLACE_GETTIMEOFDAY = 1; then AC_LIBOBJ([gettimeofday]) gl_PREREQ_GETTIMEOFDAY fi gl_SYS_TIME_MODULE_INDICATOR([gettimeofday]) gl_FUNC_INET_PTON if test $HAVE_INET_PTON = 0 || test $REPLACE_INET_NTOP = 1; then AC_LIBOBJ([inet_pton]) gl_PREREQ_INET_PTON fi gl_ARPA_INET_MODULE_INDICATOR([inet_pton]) AC_C_BIGENDIAN gl_FUNC_IOCTL if test $HAVE_IOCTL = 0 || test $REPLACE_IOCTL = 1; then AC_LIBOBJ([ioctl]) fi gl_SYS_IOCTL_MODULE_INDICATOR([ioctl]) gl_FUNC_ISBLANK if test $HAVE_ISBLANK = 0; then AC_LIBOBJ([isblank]) fi gl_CTYPE_MODULE_INDICATOR([isblank]) gl_FUNC_ISNAND_NO_LIBM if test $gl_func_isnand_no_libm != yes; then AC_LIBOBJ([isnand]) gl_PREREQ_ISNAND fi gl_DOUBLE_EXPONENT_LOCATION gl_FUNC_ISNANF_NO_LIBM if test $gl_func_isnanf_no_libm != yes; then AC_LIBOBJ([isnanf]) gl_PREREQ_ISNANF fi gl_FLOAT_EXPONENT_LOCATION gl_FUNC_ISNANL_NO_LIBM if test $gl_func_isnanl_no_libm != yes; then AC_LIBOBJ([isnanl]) gl_PREREQ_ISNANL fi gl_LONG_DOUBLE_EXPONENT_LOCATION AC_REQUIRE([gl_LONG_DOUBLE_VS_DOUBLE]) AC_REQUIRE([gl_LARGEFILE]) AC_REQUIRE([gl_HEADER_SYS_SOCKET]) if test "$ac_cv_header_winsock2_h" = yes; then AC_LIBOBJ([listen]) fi gl_SYS_SOCKET_MODULE_INDICATOR([listen]) AC_CHECK_FUNCS_ONCE([newlocale]) gl_LOCALENAME AC_CHECK_FUNCS_ONCE([newlocale]) AC_REQUIRE([gl_LOCALTIME_BUFFER_DEFAULTS]) AC_LIBOBJ([localtime-buffer]) AC_CHECK_HEADERS_ONCE([semaphore.h]) gl_FUNC_LSTAT if test $REPLACE_LSTAT = 1; then AC_LIBOBJ([lstat]) gl_PREREQ_LSTAT fi gl_SYS_STAT_MODULE_INDICATOR([lstat]) gl_MALLOCA gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_JA gt_LOCALE_ZH_CN gt_LOCALE_ZH_CN gt_LOCALE_FR_UTF8 gt_LOCALE_FR_UTF8 gt_LOCALE_FR_UTF8 dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) gl_FUNC_NANOSLEEP if test $HAVE_NANOSLEEP = 0 || test $REPLACE_NANOSLEEP = 1; then AC_LIBOBJ([nanosleep]) gl_PREREQ_NANOSLEEP fi gl_TIME_MODULE_INDICATOR([nanosleep]) AC_CHECK_DECLS_ONCE([alarm]) gl_HEADER_NETINET_IN AC_PROG_MKDIR_P gt_LOCALE_FR gt_LOCALE_FR_UTF8 gl_FUNC_OPEN if test $REPLACE_OPEN = 1; then AC_LIBOBJ([open]) gl_PREREQ_OPEN fi gl_FCNTL_MODULE_INDICATOR([open]) gl_PATHMAX gl_FUNC_PERROR if test $REPLACE_PERROR = 1; then AC_LIBOBJ([perror]) fi gl_STRING_MODULE_INDICATOR([perror]) gl_FUNC_PIPE if test $HAVE_PIPE = 0; then AC_LIBOBJ([pipe]) fi gl_UNISTD_MODULE_INDICATOR([pipe]) gl_FUNC_PTHREAD_SIGMASK if test $HAVE_PTHREAD_SIGMASK = 0 || test $REPLACE_PTHREAD_SIGMASK = 1; then AC_LIBOBJ([pthread_sigmask]) gl_PREREQ_PTHREAD_SIGMASK fi gl_SIGNAL_MODULE_INDICATOR([pthread_sigmask]) gl_FUNC_PUTENV if test $REPLACE_PUTENV = 1; then AC_LIBOBJ([putenv]) gl_PREREQ_PUTENV fi gl_STDLIB_MODULE_INDICATOR([putenv]) gl_FUNC_RAISE if test $HAVE_RAISE = 0 || test $REPLACE_RAISE = 1; then AC_LIBOBJ([raise]) gl_PREREQ_RAISE fi gl_SIGNAL_MODULE_INDICATOR([raise]) dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) gl_FUNC_SELECT if test $REPLACE_SELECT = 1; then AC_LIBOBJ([select]) fi gl_SYS_SELECT_MODULE_INDICATOR([select]) AC_CHECK_HEADERS_ONCE([sys/wait.h]) gl_FUNC_SETENV if test $HAVE_SETENV = 0 || test $REPLACE_SETENV = 1; then AC_LIBOBJ([setenv]) fi gl_STDLIB_MODULE_INDICATOR([setenv]) gl_FUNC_SETLOCALE if test $REPLACE_SETLOCALE = 1; then AC_LIBOBJ([setlocale]) gl_PREREQ_SETLOCALE fi gl_LOCALE_MODULE_INDICATOR([setlocale]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_JA gt_LOCALE_ZH_CN AC_REQUIRE([gl_HEADER_SYS_SOCKET]) if test "$ac_cv_header_winsock2_h" = yes; then AC_LIBOBJ([setsockopt]) fi gl_SYS_SOCKET_MODULE_INDICATOR([setsockopt]) gl_SIGACTION if test $HAVE_SIGACTION = 0; then AC_LIBOBJ([sigaction]) gl_PREREQ_SIGACTION fi gl_SIGNAL_MODULE_INDICATOR([sigaction]) gl_SIGNAL_H gl_SIGNBIT if test $REPLACE_SIGNBIT = 1; then AC_LIBOBJ([signbitf]) AC_LIBOBJ([signbitd]) AC_LIBOBJ([signbitl]) fi gl_MATH_MODULE_INDICATOR([signbit]) AC_REQUIRE([gl_FLOAT_EXPONENT_LOCATION]) AC_REQUIRE([gl_DOUBLE_EXPONENT_LOCATION]) AC_REQUIRE([gl_LONG_DOUBLE_EXPONENT_LOCATION]) gl_SIGNALBLOCKING if test $HAVE_POSIX_SIGNALBLOCKING = 0; then AC_LIBOBJ([sigprocmask]) gl_PREREQ_SIGPROCMASK fi gl_SIGNAL_MODULE_INDICATOR([sigprocmask]) AC_CHECK_DECLS_ONCE([alarm]) AC_REQUIRE([gl_HEADER_SYS_SOCKET]) if test "$ac_cv_header_winsock2_h" = yes; then AC_LIBOBJ([socket]) fi # When this module is used, sockets may actually occur as file descriptors, # hence it is worth warning if the modules 'close' and 'ioctl' are not used. m4_ifdef([gl_UNISTD_H_DEFAULTS], [AC_REQUIRE([gl_UNISTD_H_DEFAULTS])]) m4_ifdef([gl_SYS_IOCTL_H_DEFAULTS], [AC_REQUIRE([gl_SYS_IOCTL_H_DEFAULTS])]) AC_REQUIRE([gl_PREREQ_SYS_H_WINSOCK2]) if test "$ac_cv_header_winsock2_h" = yes; then UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=1 SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS=1 fi gl_SYS_SOCKET_MODULE_INDICATOR([socket]) AC_REQUIRE([gl_SOCKETLIB]) AC_REQUIRE([gl_SOCKETS]) gl_TYPE_SOCKLEN_T gl_FUNC_STAT if test $REPLACE_STAT = 1; then AC_LIBOBJ([stat]) case "$host_os" in mingw*) AC_LIBOBJ([stat-w32]) ;; esac gl_PREREQ_STAT fi gl_SYS_STAT_MODULE_INDICATOR([stat]) gl_STAT_TIME gl_STAT_BIRTHTIME AC_REQUIRE([gt_TYPE_WCHAR_T]) AC_REQUIRE([gt_TYPE_WINT_T]) gl_FUNC_STRERROR_R if test $HAVE_DECL_STRERROR_R = 0 || test $REPLACE_STRERROR_R = 1; then AC_LIBOBJ([strerror_r]) gl_PREREQ_STRERROR_R fi gl_STRING_MODULE_INDICATOR([strerror_r]) dnl For the modules argp, error. gl_MODULE_INDICATOR([strerror_r-posix]) dnl Check for prerequisites for memory fence checks. gl_FUNC_MMAP_ANON AC_CHECK_HEADERS_ONCE([sys/mman.h]) AC_CHECK_FUNCS_ONCE([mprotect]) gl_FUNC_SYMLINK if test $HAVE_SYMLINK = 0 || test $REPLACE_SYMLINK = 1; then AC_LIBOBJ([symlink]) fi gl_UNISTD_MODULE_INDICATOR([symlink]) gl_SYS_IOCTL_H AC_PROG_MKDIR_P AC_REQUIRE([gl_HEADER_SYS_SELECT]) AC_PROG_MKDIR_P AC_REQUIRE([gl_HEADER_SYS_SOCKET]) AC_PROG_MKDIR_P AC_CHECK_FUNCS_ONCE([shutdown]) gl_HEADER_SYS_STAT_H AC_PROG_MKDIR_P gl_HEADER_SYS_TIME_H AC_PROG_MKDIR_P gl_HEADER_SYS_UIO AC_PROG_MKDIR_P gl_THREAD gl_HEADER_TIME_H gl_FUNC_UNSETENV if test $HAVE_UNSETENV = 0 || test $REPLACE_UNSETENV = 1; then AC_LIBOBJ([unsetenv]) gl_PREREQ_UNSETENV fi gl_STDLIB_MODULE_INDICATOR([unsetenv]) gl_FUNC_USLEEP if test $HAVE_USLEEP = 0 || test $REPLACE_USLEEP = 1; then AC_LIBOBJ([usleep]) fi gl_UNISTD_MODULE_INDICATOR([usleep]) gt_LOCALE_FR gt_LOCALE_FR_UTF8 gt_LOCALE_JA gt_LOCALE_ZH_CN gl_FUNC_WCTOB if test $HAVE_WCTOB = 0 || test $REPLACE_WCTOB = 1; then AC_LIBOBJ([wctob]) gl_PREREQ_WCTOB fi gl_WCHAR_MODULE_INDICATOR([wctob]) gl_FUNC_WCTOMB if test $REPLACE_WCTOMB = 1; then AC_LIBOBJ([wctomb]) gl_PREREQ_WCTOMB fi gl_STDLIB_MODULE_INDICATOR([wctomb]) gl_YIELD m4_popdef([gl_MODULE_INDICATOR_CONDITION]) m4_ifval(gltests_LIBSOURCES_LIST, [ m4_syscmd([test ! -d ]m4_defn([gltests_LIBSOURCES_DIR])[ || for gl_file in ]gltests_LIBSOURCES_LIST[ ; do if test ! -r ]m4_defn([gltests_LIBSOURCES_DIR])[/$gl_file ; then echo "missing file ]m4_defn([gltests_LIBSOURCES_DIR])[/$gl_file" >&2 exit 1 fi done])dnl m4_if(m4_sysval, [0], [], [AC_FATAL([expected source file, required through AC_LIBSOURCES, not found])]) ]) m4_popdef([gltests_LIBSOURCES_DIR]) m4_popdef([gltests_LIBSOURCES_LIST]) m4_popdef([AC_LIBSOURCES]) m4_popdef([AC_REPLACE_FUNCS]) m4_popdef([AC_LIBOBJ]) AC_CONFIG_COMMANDS_PRE([ gltests_libobjs= gltests_ltlibobjs= if test -n "$gltests_LIBOBJS"; then # Remove the extension. sed_drop_objext='s/\.o$//;s/\.obj$//' for i in `for i in $gltests_LIBOBJS; do echo "$i"; done | sed -e "$sed_drop_objext" | sort | uniq`; do gltests_libobjs="$gltests_libobjs $i.$ac_objext" gltests_ltlibobjs="$gltests_ltlibobjs $i.lo" done fi AC_SUBST([gltests_LIBOBJS], [$gltests_libobjs]) AC_SUBST([gltests_LTLIBOBJS], [$gltests_ltlibobjs]) ]) LIBTESTS_LIBDEPS="$gltests_libdeps" AC_SUBST([LIBTESTS_LIBDEPS]) ]) # Like AC_LIBOBJ, except that the module name goes # into gl_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gl_LIBOBJ], [ AS_LITERAL_IF([$1], [gl_LIBSOURCES([$1.c])])dnl gl_LIBOBJS="$gl_LIBOBJS $1.$ac_objext" ]) # Like AC_REPLACE_FUNCS, except that the module name goes # into gl_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gl_REPLACE_FUNCS], [ m4_foreach_w([gl_NAME], [$1], [AC_LIBSOURCES(gl_NAME[.c])])dnl AC_CHECK_FUNCS([$1], , [gl_LIBOBJ($ac_func)]) ]) # Like AC_LIBSOURCES, except the directory where the source file is # expected is derived from the gnulib-tool parameterization, # and alloca is special cased (for the alloca-opt module). # We could also entirely rely on EXTRA_lib..._SOURCES. AC_DEFUN([gl_LIBSOURCES], [ m4_foreach([_gl_NAME], [$1], [ m4_if(_gl_NAME, [alloca.c], [], [ m4_define([gl_LIBSOURCES_DIR], [bootstrapped/lib]) m4_append([gl_LIBSOURCES_LIST], _gl_NAME, [ ]) ]) ]) ]) # Like AC_LIBOBJ, except that the module name goes # into gltests_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gltests_LIBOBJ], [ AS_LITERAL_IF([$1], [gltests_LIBSOURCES([$1.c])])dnl gltests_LIBOBJS="$gltests_LIBOBJS $1.$ac_objext" ]) # Like AC_REPLACE_FUNCS, except that the module name goes # into gltests_LIBOBJS instead of into LIBOBJS. AC_DEFUN([gltests_REPLACE_FUNCS], [ m4_foreach_w([gl_NAME], [$1], [AC_LIBSOURCES(gl_NAME[.c])])dnl AC_CHECK_FUNCS([$1], , [gltests_LIBOBJ($ac_func)]) ]) # Like AC_LIBSOURCES, except the directory where the source file is # expected is derived from the gnulib-tool parameterization, # and alloca is special cased (for the alloca-opt module). # We could also entirely rely on EXTRA_lib..._SOURCES. AC_DEFUN([gltests_LIBSOURCES], [ m4_foreach([_gl_NAME], [$1], [ m4_if(_gl_NAME, [alloca.c], [], [ m4_define([gltests_LIBSOURCES_DIR], [bootstrapped/tests]) m4_append([gltests_LIBSOURCES_LIST], _gl_NAME, [ ]) ]) ]) ]) # This macro records the list of files which have been installed by # gnulib-tool and may be removed by future gnulib-tool invocations. AC_DEFUN([gl_FILE_LIST], [ build-aux/config.rpath build-aux/gendocs.sh build-aux/git-version-gen doc/fdl.texi doc/gendocs_template doc/gendocs_template_min lib/_Noreturn.h lib/alloca.c lib/alloca.in.h lib/arg-nonnull.h lib/argp-ba.c lib/argp-eexst.c lib/argp-fmtstream.c lib/argp-fmtstream.h lib/argp-fs-xinl.c lib/argp-help.c lib/argp-namefrob.h lib/argp-parse.c lib/argp-pin.c lib/argp-pv.c lib/argp-pvh.c lib/argp-xinl.c lib/argp.h lib/asnprintf.c lib/basename-lgpl.c lib/btowc.c lib/c++defs.h lib/c-ctype.c lib/c-ctype.h lib/config.charset lib/dirname-lgpl.c lib/dirname.h lib/dosname.h lib/errno.in.h lib/error.c lib/error.h lib/float+.h lib/float.c lib/float.in.h lib/getdelim.c lib/getline.c lib/getopt-cdefs.in.h lib/getopt-core.h lib/getopt-ext.h lib/getopt-pfx-core.h lib/getopt-pfx-ext.h lib/getopt.c lib/getopt.in.h lib/getopt1.c lib/getopt_int.h lib/getprogname.c lib/getprogname.h lib/gettext.h lib/glthread/lock.c lib/glthread/lock.h lib/glthread/threadlib.c lib/hard-locale.c lib/hard-locale.h lib/intprops.h lib/inttypes.in.h lib/iswblank.c lib/itold.c lib/langinfo.in.h lib/limits.in.h lib/localcharset.c lib/localcharset.h lib/locale.in.h lib/localeconv.c lib/malloc.c lib/math.c lib/math.in.h lib/mbchar.c lib/mbchar.h lib/mbrtowc.c lib/mbschr.c lib/mbsinit.c lib/mbspbrk.c lib/mbsspn.c lib/mbstok_r.c lib/mbtowc-impl.h lib/mbtowc.c lib/mbuiter.c lib/mbuiter.h lib/memchr.c lib/memchr.valgrind lib/mempcpy.c lib/minmax.h lib/msvc-inval.c lib/msvc-inval.h lib/msvc-nothrow.c lib/msvc-nothrow.h lib/nl_langinfo.c lib/nproc.c lib/nproc.h lib/printf-args.c lib/printf-args.h lib/printf-parse.c lib/printf-parse.h lib/rawmemchr.c lib/rawmemchr.valgrind lib/ref-add.sin lib/ref-del.sin lib/regcomp.c lib/regex.c lib/regex.h lib/regex_internal.c lib/regex_internal.h lib/regexec.c lib/size_max.h lib/sleep.c lib/stdalign.in.h lib/stdbool.in.h lib/stddef.in.h lib/stdint.in.h lib/stdio.in.h lib/stdlib.in.h lib/strcasecmp.c lib/strchrnul.c lib/strchrnul.valgrind lib/streq.h lib/strerror-override.c lib/strerror-override.h lib/strerror.c lib/string.in.h lib/strings.in.h lib/stripslash.c lib/strncasecmp.c lib/strndup.c lib/strnlen.c lib/strnlen1.c lib/strnlen1.h lib/strtod.c lib/strtok_r.c lib/sys_types.in.h lib/sysexits.in.h lib/unistd.c lib/unistd.in.h lib/unitypes.in.h lib/uniwidth.in.h lib/uniwidth/cjk.h lib/uniwidth/width.c lib/vasnprintf.c lib/vasnprintf.h lib/verify.h lib/vsnprintf.c lib/warn-on-use.h lib/wchar.in.h lib/wcrtomb.c lib/wctype-h.c lib/wctype.in.h lib/wcwidth.c lib/xsize.c lib/xsize.h m4/00gnulib.m4 m4/absolute-header.m4 m4/alloca.m4 m4/argp.m4 m4/arpa_inet_h.m4 m4/asm-underscore.m4 m4/btowc.m4 m4/builtin-expect.m4 m4/close.m4 m4/codeset.m4 m4/configmake.m4 m4/ctype.m4 m4/dirname.m4 m4/double-slash-root.m4 m4/dup2.m4 m4/eealloc.m4 m4/environ.m4 m4/errno_h.m4 m4/error.m4 m4/exponentd.m4 m4/exponentf.m4 m4/exponentl.m4 m4/extensions.m4 m4/extern-inline.m4 m4/fcntl-o.m4 m4/fcntl.m4 m4/fcntl_h.m4 m4/fdopen.m4 m4/flexmember.m4 m4/float_h.m4 m4/fpieee.m4 m4/fstat.m4 m4/ftruncate.m4 m4/func.m4 m4/getcwd.m4 m4/getdelim.m4 m4/getdtablesize.m4 m4/getline.m4 m4/getopt.m4 m4/getpagesize.m4 m4/getprogname.m4 m4/gettimeofday.m4 m4/glibc21.m4 m4/gnulib-common.m4 m4/hard-locale.m4 m4/host-cpu-c-abi.m4 m4/include_next.m4 m4/inet_pton.m4 m4/intlmacosx.m4 m4/intmax_t.m4 m4/inttypes-pri.m4 m4/inttypes.m4 m4/inttypes_h.m4 m4/ioctl.m4 m4/isblank.m4 m4/isnand.m4 m4/isnanf.m4 m4/isnanl.m4 m4/iswblank.m4 m4/langinfo_h.m4 m4/largefile.m4 m4/lcmessage.m4 m4/ldexp.m4 m4/lib-ld.m4 m4/lib-link.m4 m4/lib-prefix.m4 m4/libunistring-base.m4 m4/limits-h.m4 m4/localcharset.m4 m4/locale-fr.m4 m4/locale-ja.m4 m4/locale-tr.m4 m4/locale-zh.m4 m4/locale_h.m4 m4/localeconv.m4 m4/localename.m4 m4/localtime-buffer.m4 m4/lock.m4 m4/longlong.m4 m4/lstat.m4 m4/malloc.m4 m4/malloca.m4 m4/math_h.m4 m4/mbchar.m4 m4/mbiter.m4 m4/mbrtowc.m4 m4/mbsinit.m4 m4/mbstate_t.m4 m4/mbtowc.m4 m4/memchr.m4 m4/mempcpy.m4 m4/minmax.m4 m4/mmap-anon.m4 m4/mode_t.m4 m4/msvc-inval.m4 m4/msvc-nothrow.m4 m4/multiarch.m4 m4/nanosleep.m4 m4/netinet_in_h.m4 m4/nl_langinfo.m4 m4/nocrash.m4 m4/nproc.m4 m4/off_t.m4 m4/open-cloexec.m4 m4/open.m4 m4/pathmax.m4 m4/perror.m4 m4/pipe.m4 m4/printf.m4 m4/pthread_rwlock_rdlock.m4 m4/pthread_sigmask.m4 m4/putenv.m4 m4/raise.m4 m4/rawmemchr.m4 m4/regex.m4 m4/select.m4 m4/setenv.m4 m4/setlocale.m4 m4/sigaction.m4 m4/signal_h.m4 m4/signalblocking.m4 m4/signbit.m4 m4/size_max.m4 m4/sleep.m4 m4/socketlib.m4 m4/sockets.m4 m4/socklen.m4 m4/sockpfaf.m4 m4/ssize_t.m4 m4/stat-time.m4 m4/stat.m4 m4/stdalign.m4 m4/stdbool.m4 m4/stddef_h.m4 m4/stdint.m4 m4/stdint_h.m4 m4/stdio_h.m4 m4/stdlib_h.m4 m4/strcase.m4 m4/strchrnul.m4 m4/strerror.m4 m4/strerror_r.m4 m4/string_h.m4 m4/strings_h.m4 m4/strndup.m4 m4/strnlen.m4 m4/strtod.m4 m4/strtok_r.m4 m4/symlink.m4 m4/sys_ioctl_h.m4 m4/sys_select_h.m4 m4/sys_socket_h.m4 m4/sys_stat_h.m4 m4/sys_time_h.m4 m4/sys_types_h.m4 m4/sys_uio_h.m4 m4/sysexits.m4 m4/thread.m4 m4/threadlib.m4 m4/time_h.m4 m4/unistd_h.m4 m4/usleep.m4 m4/vasnprintf.m4 m4/vsnprintf.m4 m4/warn-on-use.m4 m4/wchar_h.m4 m4/wchar_t.m4 m4/wcrtomb.m4 m4/wctob.m4 m4/wctomb.m4 m4/wctype_h.m4 m4/wcwidth.m4 m4/wint_t.m4 m4/xsize.m4 m4/yield.m4 tests/infinity.h tests/init.sh tests/macros.h tests/minus-zero.h tests/nan.h tests/nap.h tests/signature.h tests/test-accept.c tests/test-alloca-opt.c tests/test-argp-2.sh tests/test-argp.c tests/test-arpa_inet.c tests/test-binary-io.c tests/test-binary-io.sh tests/test-bind.c tests/test-btowc.c tests/test-btowc1.sh tests/test-btowc2.sh tests/test-c-ctype.c tests/test-c-strcase.sh tests/test-c-strcasecmp.c tests/test-c-strncasecmp.c tests/test-cloexec.c tests/test-close.c tests/test-connect.c tests/test-ctype.c tests/test-dup2.c tests/test-environ.c tests/test-errno.c tests/test-fcntl-h.c tests/test-fcntl.c tests/test-fdopen.c tests/test-fgetc.c tests/test-float.c tests/test-fputc.c tests/test-fread.c tests/test-fstat.c tests/test-ftruncate.c tests/test-ftruncate.sh tests/test-func.c tests/test-fwrite.c tests/test-getcwd-lgpl.c tests/test-getdelim.c tests/test-getdtablesize.c tests/test-getline.c tests/test-getopt-gnu.c tests/test-getopt-main.h tests/test-getopt-posix.c tests/test-getopt.h tests/test-getopt_long.h tests/test-getprogname.c tests/test-gettimeofday.c tests/test-ignore-value.c tests/test-inet_pton.c tests/test-init.sh tests/test-intprops.c tests/test-inttypes.c tests/test-ioctl.c tests/test-isblank.c tests/test-isnand-nolibm.c tests/test-isnand.h tests/test-isnanf-nolibm.c tests/test-isnanf.h tests/test-isnanl-nolibm.c tests/test-isnanl.h tests/test-iswblank.c tests/test-langinfo.c tests/test-limits-h.c tests/test-listen.c tests/test-locale.c tests/test-localeconv.c tests/test-localename.c tests/test-lock.c tests/test-lstat.c tests/test-lstat.h tests/test-malloc-gnu.c tests/test-malloca.c tests/test-math.c tests/test-mbrtowc-w32-1.sh tests/test-mbrtowc-w32-2.sh tests/test-mbrtowc-w32-3.sh tests/test-mbrtowc-w32-4.sh tests/test-mbrtowc-w32-5.sh tests/test-mbrtowc-w32.c tests/test-mbrtowc.c tests/test-mbrtowc1.sh tests/test-mbrtowc2.sh tests/test-mbrtowc3.sh tests/test-mbrtowc4.sh tests/test-mbrtowc5.sh tests/test-mbschr.c tests/test-mbschr.sh tests/test-mbsinit.c tests/test-mbsinit.sh tests/test-mbspbrk.c tests/test-mbspbrk.sh tests/test-mbsspn.c tests/test-mbsspn.sh tests/test-memchr.c tests/test-nanosleep.c tests/test-netinet_in.c tests/test-nl_langinfo.c tests/test-nl_langinfo.sh tests/test-open.c tests/test-open.h tests/test-pathmax.c tests/test-perror.c tests/test-perror.sh tests/test-perror2.c tests/test-pipe.c tests/test-pthread_sigmask1.c tests/test-pthread_sigmask2.c tests/test-raise.c tests/test-rawmemchr.c tests/test-regex.c tests/test-rwlock1.c tests/test-select-fd.c tests/test-select-in.sh tests/test-select-out.sh tests/test-select-stdin.c tests/test-select.c tests/test-select.h tests/test-setenv.c tests/test-setlocale1.c tests/test-setlocale1.sh tests/test-setlocale2.c tests/test-setlocale2.sh tests/test-setsockopt.c tests/test-sigaction.c tests/test-signal-h.c tests/test-signbit.c tests/test-sigprocmask.c tests/test-sleep.c tests/test-sockets.c tests/test-stat-time.c tests/test-stat.c tests/test-stat.h tests/test-stdalign.c tests/test-stdbool.c tests/test-stddef.c tests/test-stdint.c tests/test-stdio.c tests/test-stdlib.c tests/test-strchrnul.c tests/test-strerror.c tests/test-strerror_r.c tests/test-string.c tests/test-strings.c tests/test-strnlen.c tests/test-strtod.c tests/test-symlink.c tests/test-symlink.h tests/test-sys_ioctl.c tests/test-sys_select.c tests/test-sys_socket.c tests/test-sys_stat.c tests/test-sys_time.c tests/test-sys_types.c tests/test-sys_uio.c tests/test-sys_wait.h tests/test-sysexits.c tests/test-thread_create.c tests/test-thread_self.c tests/test-time.c tests/test-unistd.c tests/test-unsetenv.c tests/test-usleep.c tests/test-vasnprintf.c tests/test-verify-try.c tests/test-verify.c tests/test-verify.sh tests/test-vsnprintf.c tests/test-wchar.c tests/test-wcrtomb-w32-1.sh tests/test-wcrtomb-w32-2.sh tests/test-wcrtomb-w32-3.sh tests/test-wcrtomb-w32-4.sh tests/test-wcrtomb-w32-5.sh tests/test-wcrtomb-w32.c tests/test-wcrtomb.c tests/test-wcrtomb.sh tests/test-wctype-h.c tests/test-wcwidth.c tests/uniwidth/test-uc_width.c tests/uniwidth/test-uc_width2.c tests/uniwidth/test-uc_width2.sh tests/zerosize-ptr.h tests=lib/_Noreturn.h tests=lib/accept.c tests=lib/arg-nonnull.h tests=lib/arpa_inet.in.h tests=lib/binary-io.c tests=lib/binary-io.h tests=lib/bind.c tests=lib/c++defs.h tests=lib/c-strcase.h tests=lib/c-strcasecmp.c tests=lib/c-strncasecmp.c tests=lib/cloexec.c tests=lib/cloexec.h tests=lib/close.c tests=lib/connect.c tests=lib/ctype.in.h tests=lib/dup2.c tests=lib/fcntl.c tests=lib/fcntl.in.h tests=lib/fd-hook.c tests=lib/fd-hook.h tests=lib/fdopen.c tests=lib/filename.h tests=lib/flexmember.h tests=lib/float+.h tests=lib/fpucw.h tests=lib/fstat.c tests=lib/ftruncate.c tests=lib/getcwd-lgpl.c tests=lib/getdtablesize.c tests=lib/getpagesize.c tests=lib/gettimeofday.c tests=lib/glthread/thread.c tests=lib/glthread/thread.h tests=lib/glthread/yield.h tests=lib/ignore-value.h tests=lib/inet_pton.c tests=lib/ioctl.c tests=lib/isblank.c tests=lib/isnan.c tests=lib/isnand-nolibm.h tests=lib/isnand.c tests=lib/isnanf-nolibm.h tests=lib/isnanf.c tests=lib/isnanl-nolibm.h tests=lib/isnanl.c tests=lib/listen.c tests=lib/localename.c tests=lib/localename.h tests=lib/localtime-buffer.c tests=lib/localtime-buffer.h tests=lib/lstat.c tests=lib/malloca.c tests=lib/malloca.h tests=lib/malloca.valgrind tests=lib/nanosleep.c tests=lib/netinet_in.in.h tests=lib/open.c tests=lib/pathmax.h tests=lib/perror.c tests=lib/pipe.c tests=lib/pthread_sigmask.c tests=lib/putenv.c tests=lib/raise.c tests=lib/same-inode.h tests=lib/select.c tests=lib/setenv.c tests=lib/setlocale.c tests=lib/setsockopt.c tests=lib/sig-handler.c tests=lib/sig-handler.h tests=lib/sigaction.c tests=lib/signal.in.h tests=lib/signbitd.c tests=lib/signbitf.c tests=lib/signbitl.c tests=lib/sigprocmask.c tests=lib/socket.c tests=lib/sockets.c tests=lib/sockets.h tests=lib/stat-time.c tests=lib/stat-time.h tests=lib/stat-w32.c tests=lib/stat-w32.h tests=lib/stat.c tests=lib/strerror_r.c tests=lib/symlink.c tests=lib/sys_ioctl.in.h tests=lib/sys_select.in.h tests=lib/sys_socket.c tests=lib/sys_socket.in.h tests=lib/sys_stat.in.h tests=lib/sys_time.in.h tests=lib/sys_uio.in.h tests=lib/time.in.h tests=lib/unsetenv.c tests=lib/usleep.c tests=lib/w32sock.h tests=lib/warn-on-use.h tests=lib/wctob.c tests=lib/wctomb-impl.h tests=lib/wctomb.c tests=lib/xalloc-oversized.h ]) gnuastro-0.5/bootstrapped/m4/gnulib-common.m40000644000175000017500000004273613217200022016200 00000000000000# gnulib-common.m4 serial 38 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # gl_COMMON # is expanded unconditionally through gnulib-tool magic. AC_DEFUN([gl_COMMON], [ dnl Use AC_REQUIRE here, so that the code is expanded once only. AC_REQUIRE([gl_00GNULIB]) AC_REQUIRE([gl_COMMON_BODY]) ]) AC_DEFUN([gl_COMMON_BODY], [ AH_VERBATIM([_Noreturn], [/* The _Noreturn keyword of C11. */ #if ! (defined _Noreturn \ || (defined __STDC_VERSION__ && 201112 <= __STDC_VERSION__)) # if (3 <= __GNUC__ || (__GNUC__ == 2 && 8 <= __GNUC_MINOR__) \ || 0x5110 <= __SUNPRO_C) # define _Noreturn __attribute__ ((__noreturn__)) # elif defined _MSC_VER && 1200 <= _MSC_VER # define _Noreturn __declspec (noreturn) # else # define _Noreturn # endif #endif ]) AH_VERBATIM([isoc99_inline], [/* Work around a bug in Apple GCC 4.0.1 build 5465: In C99 mode, it supports the ISO C 99 semantics of 'extern inline' (unlike the GNU C semantics of earlier versions), but does not display it by setting __GNUC_STDC_INLINE__. __APPLE__ && __MACH__ test for Mac OS X. __APPLE_CC__ tests for the Apple compiler and its version. __STDC_VERSION__ tests for the C99 mode. */ #if defined __APPLE__ && defined __MACH__ && __APPLE_CC__ >= 5465 && !defined __cplusplus && __STDC_VERSION__ >= 199901L && !defined __GNUC_STDC_INLINE__ # define __GNUC_STDC_INLINE__ 1 #endif]) AH_VERBATIM([unused_parameter], [/* Define as a marker that can be attached to declarations that might not be used. 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AC_DEFUN([gl_MODULE_INDICATOR_SET_VARIABLE_AUX], [ m4_if(m4_defn([gl_MODULE_INDICATOR_CONDITION]), [1], [ dnl Simplify the expression VALUE || 1 to 1. $1=1 ], [gl_MODULE_INDICATOR_SET_VARIABLE_AUX_OR([$1], [gl_MODULE_INDICATOR_CONDITION])]) ]) # gl_MODULE_INDICATOR_SET_VARIABLE_AUX_OR([variable], [condition]) # modifies the shell variable to include the given condition. The shell # variable's value is a C preprocessor expression that evaluates to 0 or 1. 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AC_DEFUN([gl_ASSERT_NO_GNULIB_POSIXCHECK], [ dnl Override gl_WARN_ON_USE_PREPARE. dnl But hide this definition from 'aclocal'. AC_DEFUN([gl_W][ARN_ON_USE_PREPARE], []) ]) # gl_ASSERT_NO_GNULIB_TESTS # asserts that there will be no gnulib tests in the scope of the configure.ac # and thereby enables an optimization of config.h. # Used by Emacs. AC_DEFUN([gl_ASSERT_NO_GNULIB_TESTS], [ dnl Override gl_MODULE_INDICATOR_FOR_TESTS. AC_DEFUN([gl_MODULE_INDICATOR_FOR_TESTS], []) ]) # Test whether exists. # Set HAVE_FEATURES_H. AC_DEFUN([gl_FEATURES_H], [ AC_CHECK_HEADERS_ONCE([features.h]) if test $ac_cv_header_features_h = yes; then HAVE_FEATURES_H=1 else HAVE_FEATURES_H=0 fi AC_SUBST([HAVE_FEATURES_H]) ]) # m4_foreach_w # is a backport of autoconf-2.59c's m4_foreach_w. # Remove this macro when we can assume autoconf >= 2.60. m4_ifndef([m4_foreach_w], [m4_define([m4_foreach_w], [m4_foreach([$1], m4_split(m4_normalize([$2]), [ ]), [$3])])]) # AS_VAR_IF(VAR, VALUE, [IF-MATCH], [IF-NOT-MATCH]) # ---------------------------------------------------- # Backport of autoconf-2.63b's macro. # Remove this macro when we can assume autoconf >= 2.64. m4_ifndef([AS_VAR_IF], [m4_define([AS_VAR_IF], [AS_IF([test x"AS_VAR_GET([$1])" = x""$2], [$3], [$4])])]) # gl_PROG_CC_C99 # Modifies the value of the shell variable CC in an attempt to make $CC # understand ISO C99 source code. # This is like AC_PROG_CC_C99, except that # - AC_PROG_CC_C99 did not exist in Autoconf versions < 2.60, # - AC_PROG_CC_C99 does not mix well with AC_PROG_CC_STDC # , # but many more packages use AC_PROG_CC_STDC than AC_PROG_CC_C99 # . # Remaining problems: # - When AC_PROG_CC_STDC is invoked twice, it adds the C99 enabling options # to CC twice # . # - AC_PROG_CC_STDC is likely to change now that C11 is an ISO standard. 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It may seem like its easier to avoid calling the macro here, dnl but we need to AC_SUBST both AR/ARFLAGS (thus those must have some good dnl default value and automake should usually know them). dnl dnl The '][' hides this use from 'aclocal'. m4_ifdef([A][M_PROG_AR], [A][M_PROG_AR], [:]) fi dnl In case the code above has not helped with setting AR/ARFLAGS, use dnl Automake-documented default values for AR and ARFLAGS, but prefer dnl ${host}-ar over ar (useful for cross-compiling). AC_CHECK_TOOL([AR], [ar], [ar]) if test -z "$ARFLAGS"; then ARFLAGS='cr' fi AC_SUBST([AR]) AC_SUBST([ARFLAGS]) if test -z "$RANLIB"; then if test $gl_cv_c_amsterdam_compiler = yes; then RANLIB=':' else dnl Use the ranlib program if it is available. 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Do not define if restrict is supported directly. */ #undef restrict /* Work around a bug in Sun C++: it does not support _Restrict or __restrict__, even though the corresponding Sun C compiler ends up with "#define restrict _Restrict" or "#define restrict __restrict__" in the previous line. Perhaps some future version of Sun C++ will work with restrict; if so, hopefully it defines __RESTRICT like Sun C does. */ #if defined __SUNPRO_CC && !defined __RESTRICT # define _Restrict # define __restrict__ #endif]) case $ac_cv_c_restrict in restrict) ;; no) AC_DEFINE([restrict], []) ;; *) AC_DEFINE_UNQUOTED([restrict], [$ac_cv_c_restrict]) ;; esac ])# AC_C_RESTRICT # gl_BIGENDIAN # is like AC_C_BIGENDIAN, except that it can be AC_REQUIREd. # Note that AC_REQUIRE([AC_C_BIGENDIAN]) does not work reliably because some # macros invoke AC_C_BIGENDIAN with arguments. AC_DEFUN([gl_BIGENDIAN], [ AC_C_BIGENDIAN ]) # gl_CACHE_VAL_SILENT(cache-id, command-to-set-it) # is like AC_CACHE_VAL(cache-id, command-to-set-it), except that it does not # output a spurious "(cached)" mark in the midst of other configure output. # This macro should be used instead of AC_CACHE_VAL when it is not surrounded # by an AC_MSG_CHECKING/AC_MSG_RESULT pair. AC_DEFUN([gl_CACHE_VAL_SILENT], [ saved_as_echo_n="$as_echo_n" as_echo_n=':' AC_CACHE_VAL([$1], [$2]) as_echo_n="$saved_as_echo_n" ]) # AS_VAR_COPY was added in autoconf 2.63b m4_define_default([AS_VAR_COPY], [AS_LITERAL_IF([$1[]$2], [$1=$$2], [eval $1=\$$2])]) # AC_PROG_SED was added in autoconf 2.59b m4_ifndef([AC_PROG_SED], [AC_DEFUN([AC_PROG_SED], [AC_CACHE_CHECK([for a sed that does not truncate output], ac_cv_path_SED, [dnl ac_script should not contain more than 99 commands (for HP-UX sed), dnl but more than about 7000 bytes, to catch a limit in Solaris 8 /usr/ucb/sed. ac_script=s/aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa/bbbbbbbbbbbbbbbbbbbbbbbbbbbbbbbbb/ for ac_i in 1 2 3 4 5 6 7; do ac_script="$ac_script$as_nl$ac_script" done echo "$ac_script" 2>/dev/null | sed 99q >conftest.sed AS_UNSET([ac_script]) if test -z "$SED"; then ac_path_SED_found=false _AS_PATH_WALK([], [ for ac_prog in sed gsed; do for ac_exec_ext in '' $ac_executable_extensions; do ac_path_SED="$as_dir/$ac_prog$ac_exec_ext" AS_EXECUTABLE_P(["$ac_path_SED"]) || continue case `"$ac_path_SED" --version 2>&1` in *GNU*) ac_cv_path_SED=$ac_path_SED ac_path_SED_found=:;; *) ac_count=0 _AS_ECHO_N([0123456789]) >conftest.in while : do cat conftest.in conftest.in >conftest.tmp mv conftest.tmp conftest.in cp conftest.in conftest.nl echo >> conftest.nl "$ac_path_SED" -f conftest.sed conftest.out 2>/dev/null || break diff conftest.out conftest.nl >/dev/null 2>&1 || break ac_count=`expr $ac_count + 1` if test $ac_count -gt ${ac_path_SED_max-0}; then # Best so far, but keep looking for better ac_cv_path_SED=$ac_path_SED ac_path_SED_max=$ac_count fi test $ac_count -gt 10 && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out;; esac $ac_path_SED_found && break 3 done done]) if test -z "$ac_cv_path_SED"; then AC_ERROR([no acceptable sed could be found in \$PATH]) fi else ac_cv_path_SED=$SED fi ]) SED="$ac_cv_path_SED" AC_SUBST([SED])dnl rm -f conftest.sed ]) ]) gnuastro-0.5/bootstrapped/m4/glibc21.m40000644000175000017500000000161313217200022014642 00000000000000# glibc21.m4 serial 5 dnl Copyright (C) 2000-2002, 2004, 2008, 2010-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Test for the GNU C Library, version 2.1 or newer, or uClibc. # From Bruno Haible. AC_DEFUN([gl_GLIBC21], [ AC_CACHE_CHECK([whether we are using the GNU C Library >= 2.1 or uClibc], [ac_cv_gnu_library_2_1], [AC_EGREP_CPP([Lucky], [ #include #ifdef __GNU_LIBRARY__ #if (__GLIBC__ == 2 && __GLIBC_MINOR__ >= 1) || (__GLIBC__ > 2) Lucky GNU user #endif #endif #ifdef __UCLIBC__ Lucky user #endif ], [ac_cv_gnu_library_2_1=yes], [ac_cv_gnu_library_2_1=no]) ] ) AC_SUBST([GLIBC21]) GLIBC21="$ac_cv_gnu_library_2_1" ] ) gnuastro-0.5/bootstrapped/m4/gettimeofday.m40000644000175000017500000001103313217200022016075 00000000000000# serial 24 # Copyright (C) 2001-2003, 2005, 2007, 2009-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. dnl From Jim Meyering. AC_DEFUN([gl_FUNC_GETTIMEOFDAY], [ AC_REQUIRE([gl_HEADER_SYS_TIME_H_DEFAULTS]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_HEADER_SYS_TIME_H]) AC_CHECK_FUNCS_ONCE([gettimeofday]) gl_gettimeofday_timezone=void if test $ac_cv_func_gettimeofday != yes; then HAVE_GETTIMEOFDAY=0 else gl_FUNC_GETTIMEOFDAY_CLOBBER AC_CACHE_CHECK([for gettimeofday with POSIX signature], [gl_cv_func_gettimeofday_posix_signature], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include struct timeval c; int gettimeofday (struct timeval *restrict, void *restrict); ]], [[/* glibc uses struct timezone * rather than the POSIX void * if _GNU_SOURCE is defined. However, since the only portable use of gettimeofday uses NULL as the second parameter, and since the glibc definition is actually more typesafe, it is not worth wrapping this to get a compliant signature. */ int (*f) (struct timeval *restrict, void *restrict) = gettimeofday; int x = f (&c, 0); return !(x | c.tv_sec | c.tv_usec); ]])], [gl_cv_func_gettimeofday_posix_signature=yes], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include int gettimeofday (struct timeval *restrict, struct timezone *restrict); ]])], [gl_cv_func_gettimeofday_posix_signature=almost], [gl_cv_func_gettimeofday_posix_signature=no])])]) if test $gl_cv_func_gettimeofday_posix_signature = almost; then gl_gettimeofday_timezone='struct timezone' elif test $gl_cv_func_gettimeofday_posix_signature != yes; then REPLACE_GETTIMEOFDAY=1 fi dnl If we override 'struct timeval', we also have to override gettimeofday. if test $REPLACE_STRUCT_TIMEVAL = 1; then REPLACE_GETTIMEOFDAY=1 fi dnl On mingw, the original gettimeofday has only a precision of 15.6 dnl milliseconds. So override it. case "$host_os" in mingw*) REPLACE_GETTIMEOFDAY=1 ;; esac fi AC_DEFINE_UNQUOTED([GETTIMEOFDAY_TIMEZONE], [$gl_gettimeofday_timezone], [Define this to 'void' or 'struct timezone' to match the system's declaration of the second argument to gettimeofday.]) ]) dnl See if gettimeofday clobbers the static buffer that localtime uses dnl for its return value. The gettimeofday function from Mac OS X 10.0.4 dnl (i.e., Darwin 1.3.7) has this problem. dnl dnl If it does, then arrange to use gettimeofday and localtime only via dnl the wrapper functions that work around the problem. AC_DEFUN([gl_FUNC_GETTIMEOFDAY_CLOBBER], [ AC_REQUIRE([gl_HEADER_SYS_TIME_H]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([gl_LOCALTIME_BUFFER_DEFAULTS]) AC_CACHE_CHECK([whether gettimeofday clobbers localtime buffer], [gl_cv_func_gettimeofday_clobber], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include #include ]], [[ time_t t = 0; struct tm *lt; struct tm saved_lt; struct timeval tv; lt = localtime (&t); saved_lt = *lt; gettimeofday (&tv, NULL); return memcmp (lt, &saved_lt, sizeof (struct tm)) != 0; ]])], [gl_cv_func_gettimeofday_clobber=no], [gl_cv_func_gettimeofday_clobber=yes], [# When cross-compiling: case "$host_os" in # Guess all is fine on glibc systems. *-gnu*) gl_cv_func_gettimeofday_clobber="guessing no" ;; # Guess no on native Windows. mingw*) gl_cv_func_gettimeofday_clobber="guessing no" ;; # If we don't know, assume the worst. *) gl_cv_func_gettimeofday_clobber="guessing yes" ;; esac ])]) case "$gl_cv_func_gettimeofday_clobber" in *yes) REPLACE_GETTIMEOFDAY=1 AC_DEFINE([GETTIMEOFDAY_CLOBBERS_LOCALTIME], [1], [Define if gettimeofday clobbers the localtime buffer.]) gl_LOCALTIME_BUFFER_NEEDED ;; esac ]) # Prerequisites of lib/gettimeofday.c. AC_DEFUN([gl_PREREQ_GETTIMEOFDAY], [:]) gnuastro-0.5/bootstrapped/m4/getprogname.m40000644000175000017500000000263313217200022015732 00000000000000# getprogname.m4 - check for getprogname or replacements for it # Copyright (C) 2016-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # serial 4 AC_DEFUN([gl_FUNC_GETPROGNAME], [ AC_CHECK_FUNCS_ONCE([getprogname getexecname]) AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) ac_found=0 AC_CHECK_DECLS([program_invocation_name], [ac_found=1], [], [#include ]) AC_CHECK_DECLS([program_invocation_short_name], [ac_found=1], [], [#include ]) AC_CHECK_DECLS([__argv], [ac_found=1], [], [#include ]) # Incur the cost of this test only if none of the above worked. if test $ac_found = 0; then # On OpenBSD 5.1, using the global __progname variable appears to be # the only way to implement getprogname. AC_CACHE_CHECK([whether __progname is defined in default libraries], [gl_cv_var___progname], [ gl_cv_var___progname= AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[extern char *__progname;]], [[return *__progname;]] )], [gl_cv_var___progname=yes] ) ] ) if test "$gl_cv_var___progname" = yes; then AC_DEFINE([HAVE_VAR___PROGNAME], 1, [Define if you have a global __progname variable]) fi fi ]) gnuastro-0.5/bootstrapped/m4/getpagesize.m40000644000175000017500000000172213217200022015727 00000000000000# getpagesize.m4 serial 9 dnl Copyright (C) 2002, 2004-2005, 2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_GETPAGESIZE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS([getpagesize]) if test $ac_cv_func_getpagesize = no; then HAVE_GETPAGESIZE=0 AC_CHECK_HEADERS([OS.h]) if test $ac_cv_header_OS_h = yes; then HAVE_OS_H=1 fi AC_CHECK_HEADERS([sys/param.h]) if test $ac_cv_header_sys_param_h = yes; then HAVE_SYS_PARAM_H=1 fi fi case "$host_os" in mingw*) REPLACE_GETPAGESIZE=1 ;; esac dnl Also check whether it's declared. dnl mingw has getpagesize() in libgcc.a but doesn't declare it. AC_CHECK_DECL([getpagesize], , [HAVE_DECL_GETPAGESIZE=0]) ]) gnuastro-0.5/bootstrapped/m4/getopt.m40000644000175000017500000003131113217200022014717 00000000000000# getopt.m4 serial 46 dnl Copyright (C) 2002-2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Request a POSIX compliant getopt function. AC_DEFUN([gl_FUNC_GETOPT_POSIX], [ m4_divert_text([DEFAULTS], [gl_getopt_required=POSIX]) AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_GETOPT_CHECK_HEADERS]) dnl Other modules can request the gnulib implementation of the getopt dnl functions unconditionally, by defining gl_REPLACE_GETOPT_ALWAYS. dnl argp.m4 does this. m4_ifdef([gl_REPLACE_GETOPT_ALWAYS], [ REPLACE_GETOPT=1 ], [ REPLACE_GETOPT=0 if test -n "$gl_replace_getopt"; then REPLACE_GETOPT=1 fi ]) if test $REPLACE_GETOPT = 1; then dnl Arrange for getopt.h to be created. gl_GETOPT_SUBSTITUTE_HEADER fi ]) # Request a POSIX compliant getopt function with GNU extensions (such as # options with optional arguments) and the functions getopt_long, # getopt_long_only. AC_DEFUN([gl_FUNC_GETOPT_GNU], [ dnl Set the variable gl_getopt_required, so that all invocations of dnl gl_GETOPT_CHECK_HEADERS in the scope of the current configure file dnl will check for getopt with GNU extensions. dnl This means that if one gnulib-tool invocation requests getopt-posix dnl and another gnulib-tool invocation requests getopt-gnu, it is as if dnl both had requested getopt-gnu. m4_divert_text([INIT_PREPARE], [gl_getopt_required=GNU]) dnl No need to invoke gl_FUNC_GETOPT_POSIX here; this is automatically dnl done through the module dependency getopt-gnu -> getopt-posix. ]) # Determine whether to replace the entire getopt facility. AC_DEFUN([gl_GETOPT_CHECK_HEADERS], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_REQUIRE([AC_PROG_AWK]) dnl for awk that supports ENVIRON dnl Persuade Solaris to declare optarg, optind, opterr, optopt. AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) gl_CHECK_NEXT_HEADERS([getopt.h]) if test $ac_cv_header_getopt_h = yes; then HAVE_GETOPT_H=1 else HAVE_GETOPT_H=0 fi AC_SUBST([HAVE_GETOPT_H]) gl_replace_getopt= dnl Test whether is available. if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then AC_CHECK_HEADERS([getopt.h], [], [gl_replace_getopt=yes]) fi dnl Test whether the function getopt_long is available. if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then AC_CHECK_FUNCS([getopt_long_only], [], [gl_replace_getopt=yes]) fi dnl POSIX 2008 does not specify leading '+' behavior, but see dnl http://austingroupbugs.net/view.php?id=191 for a recommendation on dnl the next version of POSIX. For now, we only guarantee leading '+' dnl behavior with getopt-gnu. if test -z "$gl_replace_getopt"; then AC_CACHE_CHECK([whether getopt is POSIX compatible], [gl_cv_func_getopt_posix], [ dnl Merging these three different test programs into a single one dnl would require a reset mechanism. On BSD systems, it can be done dnl through 'optreset'; on some others (glibc), it can be done by dnl setting 'optind' to 0; on others again (HP-UX, IRIX, OSF/1, dnl Solaris 9, musl libc), there is no such mechanism. if test $cross_compiling = no; then dnl Sanity check. Succeeds everywhere (except on MSVC, dnl which lacks and getopt() entirely). AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { static char program[] = "program"; static char a[] = "-a"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, a, foo, bar, NULL }; int c; c = getopt (4, argv, "ab"); if (!(c == 'a')) return 1; c = getopt (4, argv, "ab"); if (!(c == -1)) return 2; if (!(optind == 2)) return 3; return 0; } ]])], [gl_cv_func_getopt_posix=maybe], [gl_cv_func_getopt_posix=no]) if test $gl_cv_func_getopt_posix = maybe; then dnl Sanity check with '+'. Succeeds everywhere (except on MSVC, dnl which lacks and getopt() entirely). AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { static char program[] = "program"; static char donald[] = "donald"; static char p[] = "-p"; static char billy[] = "billy"; static char duck[] = "duck"; static char a[] = "-a"; static char bar[] = "bar"; char *argv[] = { program, donald, p, billy, duck, a, bar, NULL }; int c; c = getopt (7, argv, "+abp:q:"); if (!(c == -1)) return 4; if (!(strcmp (argv[0], "program") == 0)) return 5; if (!(strcmp (argv[1], "donald") == 0)) return 6; if (!(strcmp (argv[2], "-p") == 0)) return 7; if (!(strcmp (argv[3], "billy") == 0)) return 8; if (!(strcmp (argv[4], "duck") == 0)) return 9; if (!(strcmp (argv[5], "-a") == 0)) return 10; if (!(strcmp (argv[6], "bar") == 0)) return 11; if (!(optind == 1)) return 12; return 0; } ]])], [gl_cv_func_getopt_posix=maybe], [gl_cv_func_getopt_posix=no]) fi if test $gl_cv_func_getopt_posix = maybe; then dnl Detect Mac OS X 10.5, AIX 7.1, mingw bug. AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include int main () { static char program[] = "program"; static char ab[] = "-ab"; char *argv[3] = { program, ab, NULL }; if (getopt (2, argv, "ab:") != 'a') return 13; if (getopt (2, argv, "ab:") != '?') return 14; if (optopt != 'b') return 15; if (optind != 2) return 16; return 0; } ]])], [gl_cv_func_getopt_posix=yes], [gl_cv_func_getopt_posix=no]) fi else case "$host_os" in darwin* | aix* | mingw*) gl_cv_func_getopt_posix="guessing no";; *) gl_cv_func_getopt_posix="guessing yes";; esac fi ]) case "$gl_cv_func_getopt_posix" in *no) gl_replace_getopt=yes ;; esac fi if test -z "$gl_replace_getopt" && test $gl_getopt_required = GNU; then AC_CACHE_CHECK([for working GNU getopt function], [gl_cv_func_getopt_gnu], [# Even with POSIXLY_CORRECT, the GNU extension of leading '-' in the # optstring is necessary for programs like m4 that have POSIX-mandated # semantics for supporting options interspersed with files. # Also, since getopt_long is a GNU extension, we require optind=0. # Bash ties 'set -o posix' to a non-exported POSIXLY_CORRECT; # so take care to revert to the correct (non-)export state. dnl GNU Coding Standards currently allow awk but not env; besides, env dnl is ambiguous with environment values that contain newlines. gl_awk_probe='BEGIN { if ("POSIXLY_CORRECT" in ENVIRON) print "x" }' case ${POSIXLY_CORRECT+x}`$AWK "$gl_awk_probe" #include #include ]GL_NOCRASH[ ]], [[ int result = 0; nocrash_init(); /* This code succeeds on glibc 2.8, OpenBSD 4.0, Cygwin, mingw, and fails on Mac OS X 10.5, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10. */ { static char conftest[] = "conftest"; static char plus[] = "-+"; char *argv[3] = { conftest, plus, NULL }; opterr = 0; if (getopt (2, argv, "+a") != '?') result |= 1; } /* This code succeeds on glibc 2.8, mingw, and fails on Mac OS X 10.5, OpenBSD 4.0, AIX 5.2, HP-UX 11, IRIX 6.5, OSF/1 5.1, Solaris 10, Cygwin 1.5.x. */ { static char program[] = "program"; static char p[] = "-p"; static char foo[] = "foo"; static char bar[] = "bar"; char *argv[] = { program, p, foo, bar, NULL }; optind = 1; if (getopt (4, argv, "p::") != 'p') result |= 2; else if (optarg != NULL) result |= 4; else if (getopt (4, argv, "p::") != -1) result |= 6; else if (optind != 2) result |= 8; } /* This code succeeds on glibc 2.8 and fails on Cygwin 1.7.0. */ { static char program[] = "program"; static char foo[] = "foo"; static char p[] = "-p"; char *argv[] = { program, foo, p, NULL }; optind = 0; if (getopt (3, argv, "-p") != 1) result |= 16; else if (getopt (3, argv, "-p") != 'p') result |= 16; } /* This code fails on glibc 2.11. */ { static char program[] = "program"; static char b[] = "-b"; static char a[] = "-a"; char *argv[] = { program, b, a, NULL }; optind = opterr = 0; if (getopt (3, argv, "+:a:b") != 'b') result |= 32; else if (getopt (3, argv, "+:a:b") != ':') result |= 32; } /* This code dumps core on glibc 2.14. */ { static char program[] = "program"; static char w[] = "-W"; static char dummy[] = "dummy"; char *argv[] = { program, w, dummy, NULL }; optind = opterr = 1; if (getopt (3, argv, "W;") != 'W') result |= 64; } return result; ]])], [gl_cv_func_getopt_gnu=yes], [gl_cv_func_getopt_gnu=no], [dnl Cross compiling. Assume the worst, even on glibc platforms. gl_cv_func_getopt_gnu="guessing no" ]) case $gl_had_POSIXLY_CORRECT in exported) ;; yes) AS_UNSET([POSIXLY_CORRECT]); POSIXLY_CORRECT=1 ;; *) AS_UNSET([POSIXLY_CORRECT]) ;; esac ]) if test "$gl_cv_func_getopt_gnu" != yes; then gl_replace_getopt=yes else AC_CACHE_CHECK([for working GNU getopt_long function], [gl_cv_func_getopt_long_gnu], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include ]], [[static const struct option long_options[] = { { "xtremely-",no_argument, NULL, 1003 }, { "xtra", no_argument, NULL, 1001 }, { "xtreme", no_argument, NULL, 1002 }, { "xtremely", no_argument, NULL, 1003 }, { NULL, 0, NULL, 0 } }; /* This code fails on OpenBSD 5.0. */ { static char program[] = "program"; static char xtremel[] = "--xtremel"; char *argv[] = { program, xtremel, NULL }; int option_index; optind = 1; opterr = 0; if (getopt_long (2, argv, "", long_options, &option_index) != 1003) return 1; } return 0; ]])], [gl_cv_func_getopt_long_gnu=yes], [gl_cv_func_getopt_long_gnu=no], [dnl Cross compiling. Guess no on OpenBSD, yes otherwise. case "$host_os" in openbsd*) gl_cv_func_getopt_long_gnu="guessing no";; *) gl_cv_func_getopt_long_gnu="guessing yes";; esac ]) ]) case "$gl_cv_func_getopt_long_gnu" in *yes) ;; *) gl_replace_getopt=yes ;; esac fi fi ]) AC_DEFUN([gl_GETOPT_SUBSTITUTE_HEADER], [ AC_CHECK_HEADERS_ONCE([sys/cdefs.h]) if test $ac_cv_header_sys_cdefs_h = yes; then HAVE_SYS_CDEFS_H=1 else HAVE_SYS_CDEFS_H=0 fi AC_SUBST([HAVE_SYS_CDEFS_H]) AC_DEFINE([__GETOPT_PREFIX], [[rpl_]], [Define to rpl_ if the getopt replacement functions and variables should be used.]) GETOPT_H=getopt.h GETOPT_CDEFS_H=getopt-cdefs.h AC_SUBST([GETOPT_H]) AC_SUBST([GETOPT_CDEFS_H]) ]) gnuastro-0.5/bootstrapped/m4/getline.m40000644000175000017500000000601313217200022015045 00000000000000# getline.m4 serial 28 dnl Copyright (C) 1998-2003, 2005-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_PREREQ([2.59]) dnl See if there's a working, system-supplied version of the getline function. dnl We can't just do AC_REPLACE_FUNCS([getline]) because some systems dnl have a function by that name in -linet that doesn't have anything dnl to do with the function we need. AC_DEFUN([gl_FUNC_GETLINE], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) dnl Persuade glibc to declare getline(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_DECLS_ONCE([getline]) gl_getline_needs_run_time_check=no AC_CHECK_FUNC([getline], [dnl Found it in some library. Verify that it works. gl_getline_needs_run_time_check=yes], [am_cv_func_working_getline=no]) if test $gl_getline_needs_run_time_check = yes; then AC_CACHE_CHECK([for working getline function], [am_cv_func_working_getline], [echo fooNbarN | tr -d '\012' | tr N '\012' > conftest.data AC_RUN_IFELSE([AC_LANG_SOURCE([[ # include # include # include int main () { FILE *in = fopen ("./conftest.data", "r"); if (!in) return 1; { /* Test result for a NULL buffer and a zero size. Based on a test program from Karl Heuer. */ char *line = NULL; size_t siz = 0; int len = getline (&line, &siz, in); if (!(len == 4 && line && strcmp (line, "foo\n") == 0)) { free (line); fclose (in); return 2; } free (line); } { /* Test result for a NULL buffer and a non-zero size. This crashes on FreeBSD 8.0. */ char *line = NULL; size_t siz = (size_t)(~0) / 4; if (getline (&line, &siz, in) == -1) { fclose (in); return 3; } free (line); } fclose (in); return 0; } ]])], [am_cv_func_working_getline=yes] dnl The library version works. , [am_cv_func_working_getline=no] dnl The library version does NOT work. , dnl We're cross compiling. Assume it works on glibc2 systems. [AC_EGREP_CPP([Lucky GNU user], [ #include #ifdef __GNU_LIBRARY__ #if (__GLIBC__ >= 2) && !defined __UCLIBC__ Lucky GNU user #endif #endif ], [am_cv_func_working_getline="guessing yes"], [am_cv_func_working_getline="guessing no"])] )]) fi if test $ac_cv_have_decl_getline = no; then HAVE_DECL_GETLINE=0 fi case "$am_cv_func_working_getline" in *no) dnl Set REPLACE_GETLINE always: Even if we have not found the broken dnl getline function among $LIBS, it may exist in libinet and the dnl executable may be linked with -linet. REPLACE_GETLINE=1 ;; esac ]) # Prerequisites of lib/getline.c. AC_DEFUN([gl_PREREQ_GETLINE], [ : ]) gnuastro-0.5/bootstrapped/m4/getdtablesize.m40000644000175000017500000000474013217200022016251 00000000000000# getdtablesize.m4 serial 7 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_GETDTABLESIZE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS_ONCE([getdtablesize]) AC_CHECK_DECLS_ONCE([getdtablesize]) if test $ac_cv_func_getdtablesize = yes && test $ac_cv_have_decl_getdtablesize = yes; then AC_CACHE_CHECK([whether getdtablesize works], [gl_cv_func_getdtablesize_works], [dnl There are two concepts: the "maximum possible file descriptor value + 1" dnl and the "maximum number of open file descriptors in a process". dnl Per SUSv2 and POSIX, getdtablesize() should return the first one. dnl On most platforms, the first and the second concept are the same. dnl On OpenVMS, however, they are different and getdtablesize() returns dnl the second one; thus the test below fails. But we don't care dnl because there's no good way to write a replacement getdtablesize(). case "$host_os" in vms*) gl_cv_func_getdtablesize_works="no (limitation)" ;; *) dnl Cygwin 1.7.25 automatically increases the RLIMIT_NOFILE soft dnl limit up to an unchangeable hard limit; all other platforms dnl correctly require setrlimit before getdtablesize() can report dnl a larger value. AC_RUN_IFELSE([ AC_LANG_PROGRAM([[#include ]], [int size = getdtablesize(); if (dup2 (0, getdtablesize()) != -1) return 1; if (size != getdtablesize()) return 2; ])], [gl_cv_func_getdtablesize_works=yes], [gl_cv_func_getdtablesize_works=no], [case "$host_os" in cygwin*) # on cygwin 1.5.25, getdtablesize() automatically grows gl_cv_func_getdtablesize_works="guessing no" ;; *) gl_cv_func_getdtablesize_works="guessing yes" ;; esac ]) ;; esac ]) case "$gl_cv_func_getdtablesize_works" in *yes | "no (limitation)") ;; *) REPLACE_GETDTABLESIZE=1 ;; esac else HAVE_GETDTABLESIZE=0 fi ]) # Prerequisites of lib/getdtablesize.c. AC_DEFUN([gl_PREREQ_GETDTABLESIZE], [:]) gnuastro-0.5/bootstrapped/m4/getdelim.m40000644000175000017500000000504313217200022015212 00000000000000# getdelim.m4 serial 12 dnl Copyright (C) 2005-2007, 2009-2017 Free Software Foundation, Inc. dnl dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_PREREQ([2.59]) AC_DEFUN([gl_FUNC_GETDELIM], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) dnl Persuade glibc to declare getdelim(). AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) AC_CHECK_DECLS_ONCE([getdelim]) AC_CHECK_FUNCS_ONCE([getdelim]) if test $ac_cv_func_getdelim = yes; then HAVE_GETDELIM=1 dnl Found it in some library. Verify that it works. AC_CACHE_CHECK([for working getdelim function], [gl_cv_func_working_getdelim], [echo fooNbarN | tr -d '\012' | tr N '\012' > conftest.data AC_RUN_IFELSE([AC_LANG_SOURCE([[ # include # include # include int main () { FILE *in = fopen ("./conftest.data", "r"); if (!in) return 1; { /* Test result for a NULL buffer and a zero size. Based on a test program from Karl Heuer. */ char *line = NULL; size_t siz = 0; int len = getdelim (&line, &siz, '\n', in); if (!(len == 4 && line && strcmp (line, "foo\n") == 0)) { free (line); fclose (in); return 2; } } { /* Test result for a NULL buffer and a non-zero size. This crashes on FreeBSD 8.0. */ char *line = NULL; size_t siz = (size_t)(~0) / 4; if (getdelim (&line, &siz, '\n', in) == -1) { fclose (in); return 3; } free (line); } fclose (in); return 0; } ]])], [gl_cv_func_working_getdelim=yes] dnl The library version works. , [gl_cv_func_working_getdelim=no] dnl The library version does NOT work. , dnl We're cross compiling. Assume it works on glibc2 systems. [AC_EGREP_CPP([Lucky GNU user], [ #include #ifdef __GNU_LIBRARY__ #if (__GLIBC__ >= 2) && !defined __UCLIBC__ Lucky GNU user #endif #endif ], [gl_cv_func_working_getdelim="guessing yes"], [gl_cv_func_working_getdelim="guessing no"])] )]) case "$gl_cv_func_working_getdelim" in *no) REPLACE_GETDELIM=1 ;; esac else HAVE_GETDELIM=0 fi if test $ac_cv_have_decl_getdelim = no; then HAVE_DECL_GETDELIM=0 fi ]) # Prerequisites of lib/getdelim.c. AC_DEFUN([gl_PREREQ_GETDELIM], [ AC_CHECK_FUNCS([flockfile funlockfile]) AC_CHECK_DECLS([getc_unlocked]) ]) gnuastro-0.5/bootstrapped/m4/getcwd.m40000644000175000017500000001172013217200022014674 00000000000000# getcwd.m4 - check for working getcwd that is compatible with glibc # Copyright (C) 2001, 2003-2007, 2009-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert. # serial 14 AC_DEFUN([gl_FUNC_GETCWD_NULL], [ AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_HEADERS_ONCE([unistd.h]) AC_CACHE_CHECK([whether getcwd (NULL, 0) allocates memory for result], [gl_cv_func_getcwd_null], [AC_RUN_IFELSE([AC_LANG_PROGRAM([[ # include # if HAVE_UNISTD_H # include # else /* on Windows with MSVC */ # include # endif # ifndef getcwd char *getcwd (); # endif ]], [[ #if (defined _WIN32 || defined __WIN32__) && ! defined __CYGWIN__ /* mingw cwd does not start with '/', but getcwd does allocate. However, mingw fails to honor non-zero size. */ #else if (chdir ("/") != 0) return 1; else { char *f = getcwd (NULL, 0); if (! f) return 2; if (f[0] != '/') { free (f); return 3; } if (f[1] != '\0') { free (f); return 4; } free (f); return 0; } #endif ]])], [gl_cv_func_getcwd_null=yes], [gl_cv_func_getcwd_null=no], [[case "$host_os" in # Guess yes on glibc systems. *-gnu*) gl_cv_func_getcwd_null="guessing yes";; # Guess yes on Cygwin. cygwin*) gl_cv_func_getcwd_null="guessing yes";; # If we don't know, assume the worst. *) gl_cv_func_getcwd_null="guessing no";; esac ]])]) ]) AC_DEFUN([gl_FUNC_GETCWD_SIGNATURE], [ AC_CACHE_CHECK([for getcwd with POSIX signature], [gl_cv_func_getcwd_posix_signature], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[extern #ifdef __cplusplus "C" #endif char *getcwd (char *, size_t); ]]) ], [gl_cv_func_getcwd_posix_signature=yes], [gl_cv_func_getcwd_posix_signature=no]) ]) ]) dnl Guarantee that getcwd will malloc with a NULL first argument. Assumes dnl that either the system getcwd is robust, or that calling code is okay dnl with spurious failures when run from a directory with an absolute name dnl larger than 4k bytes. dnl dnl Assumes that getcwd exists; if you are worried about obsolete dnl platforms that lacked getcwd(), then you need to use the GPL module. AC_DEFUN([gl_FUNC_GETCWD_LGPL], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_FUNC_GETCWD_NULL]) AC_REQUIRE([gl_FUNC_GETCWD_SIGNATURE]) case $gl_cv_func_getcwd_null,$gl_cv_func_getcwd_posix_signature in *yes,yes) ;; *) dnl Minimal replacement lib/getcwd-lgpl.c. REPLACE_GETCWD=1 ;; esac ]) dnl Check for all known getcwd bugs; useful for a program likely to be dnl executed from an arbitrary location. AC_DEFUN([gl_FUNC_GETCWD], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([gl_FUNC_GETCWD_NULL]) AC_REQUIRE([gl_FUNC_GETCWD_SIGNATURE]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles gl_abort_bug=no case "$host_os" in mingw*) gl_cv_func_getcwd_path_max=yes ;; *) gl_FUNC_GETCWD_PATH_MAX case "$gl_cv_func_getcwd_null" in *yes) gl_FUNC_GETCWD_ABORT_BUG([gl_abort_bug=yes]) ;; esac ;; esac dnl Define HAVE_MINIMALLY_WORKING_GETCWD and HAVE_PARTLY_WORKING_GETCWD dnl if appropriate. case "$gl_cv_func_getcwd_path_max" in "no"|"no, it has the AIX bug") ;; *) AC_DEFINE([HAVE_MINIMALLY_WORKING_GETCWD], [1], [Define to 1 if getcwd minimally works, that is, its result can be trusted when it succeeds.]) ;; esac case "$gl_cv_func_getcwd_path_max" in "no, but it is partly working") AC_DEFINE([HAVE_PARTLY_WORKING_GETCWD], [1], [Define to 1 if getcwd works, except it sometimes fails when it shouldn't, setting errno to ERANGE, ENAMETOOLONG, or ENOENT.]) ;; "yes, but with shorter paths") AC_DEFINE([HAVE_GETCWD_SHORTER], [1], [Define to 1 if getcwd works, but with shorter paths than is generally tested with the replacement.]) ;; esac if { case "$gl_cv_func_getcwd_null" in *yes) false;; *) true;; esac; } \ || test $gl_cv_func_getcwd_posix_signature != yes \ || { case "$gl_cv_func_getcwd_path_max" in *yes*) false;; *) true;; esac; } \ || test $gl_abort_bug = yes; then REPLACE_GETCWD=1 fi ]) # Prerequisites of lib/getcwd.c, when full replacement is in effect. AC_DEFUN([gl_PREREQ_GETCWD], [ AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_CHECK_TYPE_STRUCT_DIRENT_D_INO]) : ]) gnuastro-0.5/bootstrapped/m4/func.m40000644000175000017500000000131313217200022014347 00000000000000# func.m4 serial 2 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # Written by Simon Josefsson AC_DEFUN([gl_FUNC], [ AC_CACHE_CHECK([whether __func__ is available], [gl_cv_var_func], AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[]], [[const char *str = __func__;]])], [gl_cv_var_func=yes], [gl_cv_var_func=no])) if test "$gl_cv_var_func" != yes; then AC_DEFINE([__func__], [""], [Define as a replacement for the ISO C99 __func__ variable.]) fi ]) gnuastro-0.5/bootstrapped/m4/ftruncate.m40000644000175000017500000000233313217200022015412 00000000000000# serial 20 # See if we need to emulate a missing ftruncate function using chsize. # Copyright (C) 2000-2001, 2003-2007, 2009-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_FTRUNCATE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([ftruncate]) if test $ac_cv_func_ftruncate = yes; then m4_ifdef([gl_LARGEFILE], [ AC_REQUIRE([AC_CANONICAL_HOST]) case "$host_os" in mingw*) dnl Native Windows, and Large File Support is requested. dnl The MSVCRT _chsize() function only accepts a 32-bit file size, dnl and the mingw64 ftruncate64() function is unreliable (it may dnl delete the file, see dnl ). dnl Use gnulib's ftruncate() implementation instead. REPLACE_FTRUNCATE=1 ;; esac ], [ : ]) else HAVE_FTRUNCATE=0 fi ]) # Prerequisites of lib/ftruncate.c. AC_DEFUN([gl_PREREQ_FTRUNCATE], [ AC_CHECK_FUNCS([chsize]) ]) gnuastro-0.5/bootstrapped/m4/fstat.m40000644000175000017500000000206313217200022014540 00000000000000# fstat.m4 serial 6 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_FSTAT], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([gl_SYS_STAT_H_DEFAULTS]) case "$host_os" in mingw* | solaris*) dnl On MinGW, the original stat() returns st_atime, st_mtime, dnl st_ctime values that are affected by the time zone. dnl Solaris stat can return a negative tv_nsec. REPLACE_FSTAT=1 ;; esac dnl Replace fstat() for supporting the gnulib-defined open() on directories. m4_ifdef([gl_FUNC_FCHDIR], [ gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then case "$gl_cv_func_open_directory_works" in *yes) ;; *) REPLACE_FSTAT=1 ;; esac fi ]) ]) # Prerequisites of lib/fstat.c and lib/stat-w32.c. AC_DEFUN([gl_PREREQ_FSTAT], [ AC_REQUIRE([gl_HEADER_SYS_STAT_H]) : ]) gnuastro-0.5/bootstrapped/m4/fpieee.m40000644000175000017500000000434013217200022014654 00000000000000# fpieee.m4 serial 2 -*- coding: utf-8 -*- dnl Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl IEEE 754 standardized three items: dnl - The formats of single-float and double-float - nowadays commonly dnl available as 'float' and 'double' in C and C++. dnl No autoconf test needed. dnl - The overflow and division by zero behaviour: The result are values dnl '±Inf' and 'NaN', rather than exceptions as it was before. dnl This file provides an autoconf macro for ensuring this behaviour of dnl floating-point operations. dnl - A set of conditions (overflow, underflow, inexact, etc.) which can dnl be configured to trigger an exception. dnl This cannot be done in a portable way: it depends on the compiler, dnl libc, kernel, and CPU. No autoconf macro is provided for this. dnl Ensure non-trapping behaviour of floating-point overflow and dnl floating-point division by zero. dnl (For integer overflow, see gcc's -ftrapv option; for integer division by dnl zero, see the autoconf macro in intdiv0.m4.) AC_DEFUN([gl_FP_IEEE], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) # IEEE behaviour is the default on all CPUs except Alpha and SH # (according to the test results of Bruno Haible's ieeefp/fenv_default.m4 # and the GCC 4.1.2 manual). case "$host_cpu" in alpha*) # On Alpha systems, a compiler option provides the behaviour. # See the ieee(3) manual page, also available at # if test -n "$GCC"; then # GCC has the option -mieee. # For full IEEE compliance (rarely needed), use option -mieee-with-inexact. CPPFLAGS="$CPPFLAGS -mieee" else # Compaq (ex-DEC) C has the option -ieee, equivalent to -ieee_with_no_inexact. # For full IEEE compliance (rarely needed), use option -ieee_with_inexact. CPPFLAGS="$CPPFLAGS -ieee" fi ;; sh*) if test -n "$GCC"; then # GCC has the option -mieee. CPPFLAGS="$CPPFLAGS -mieee" fi ;; esac ]) gnuastro-0.5/bootstrapped/m4/float_h.m40000644000175000017500000000545713217200022015045 00000000000000# float_h.m4 serial 12 dnl Copyright (C) 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FLOAT_H], [ AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_CANONICAL_HOST]) FLOAT_H= REPLACE_FLOAT_LDBL=0 case "$host_os" in aix* | beos* | openbsd* | mirbsd* | irix*) FLOAT_H=float.h ;; freebsd* | dragonfly*) case "$host_cpu" in changequote(,)dnl i[34567]86 ) changequote([,])dnl FLOAT_H=float.h ;; x86_64 ) # On x86_64 systems, the C compiler may still be generating # 32-bit code. AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __LP64__ || defined __x86_64__ || defined __amd64__ int ok; #else error fail #endif ]])], [], [FLOAT_H=float.h]) ;; esac ;; linux*) case "$host_cpu" in powerpc*) FLOAT_H=float.h ;; esac ;; esac case "$host_os" in aix* | freebsd* | dragonfly* | linux*) if test -n "$FLOAT_H"; then REPLACE_FLOAT_LDBL=1 fi ;; esac dnl Test against glibc-2.7 Linux/SPARC64 bug. REPLACE_ITOLD=0 AC_CACHE_CHECK([whether conversion from 'int' to 'long double' works], [gl_cv_func_itold_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ int i = -1; volatile long double ld; int main () { ld += i * 1.0L; if (ld > 0) return 1; return 0; }]])], [gl_cv_func_itold_works=yes], [gl_cv_func_itold_works=no], [case "$host" in sparc*-*-linux*) AC_COMPILE_IFELSE( [AC_LANG_SOURCE( [[#if defined __LP64__ || defined __arch64__ int ok; #else error fail #endif ]])], [gl_cv_func_itold_works="guessing no"], [gl_cv_func_itold_works="guessing yes"]) ;; # Guess yes on native Windows. mingw*) gl_cv_func_itold_works="guessing yes" ;; *) gl_cv_func_itold_works="guessing yes" ;; esac ]) ]) case "$gl_cv_func_itold_works" in *no) REPLACE_ITOLD=1 dnl We add the workaround to but also to , dnl to increase the chances that the fix function gets pulled in. FLOAT_H=float.h ;; esac if test -n "$FLOAT_H"; then gl_NEXT_HEADERS([float.h]) fi AC_SUBST([FLOAT_H]) AM_CONDITIONAL([GL_GENERATE_FLOAT_H], [test -n "$FLOAT_H"]) AC_SUBST([REPLACE_ITOLD]) ]) gnuastro-0.5/bootstrapped/m4/flexmember.m40000644000175000017500000000345313217200022015551 00000000000000# serial 5 # Check for flexible array member support. # Copyright (C) 2006, 2009-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # Written by Paul Eggert. AC_DEFUN([AC_C_FLEXIBLE_ARRAY_MEMBER], [ AC_CACHE_CHECK([for flexible array member], ac_cv_c_flexmember, [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include struct m { struct m *next, **list; char name[]; }; struct s { struct s *p; struct m *m; int n; double d[]; };]], [[int m = getchar (); size_t nbytes = offsetof (struct s, d) + m * sizeof (double); nbytes += sizeof (struct s) - 1; nbytes -= nbytes % sizeof (struct s); struct s *p = malloc (nbytes); p->p = p; p->m = NULL; p->d[0] = 0.0; return p->d != (double *) NULL;]])], [ac_cv_c_flexmember=yes], [ac_cv_c_flexmember=no])]) if test $ac_cv_c_flexmember = yes; then AC_DEFINE([FLEXIBLE_ARRAY_MEMBER], [], [Define to nothing if C supports flexible array members, and to 1 if it does not. That way, with a declaration like 'struct s { int n; double d@<:@FLEXIBLE_ARRAY_MEMBER@:>@; };', the struct hack can be used with pre-C99 compilers. When computing the size of such an object, don't use 'sizeof (struct s)' as it overestimates the size. Use 'offsetof (struct s, d)' instead. Don't use 'offsetof (struct s, d@<:@0@:>@)', as this doesn't work with MSVC and with C++ compilers.]) else AC_DEFINE([FLEXIBLE_ARRAY_MEMBER], [1]) fi ]) gnuastro-0.5/bootstrapped/m4/fdopen.m40000644000175000017500000000257613217200022014703 00000000000000# fdopen.m4 serial 4 dnl Copyright (C) 2011-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_FDOPEN], [ AC_REQUIRE([gl_STDIO_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles m4_ifdef([gl_MSVC_INVAL], [ AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_FDOPEN=1 fi ]) if test $REPLACE_FDOPEN = 0; then dnl Test whether fdopen() sets errno when it fails due to a bad fd argument. AC_CACHE_CHECK([whether fdopen sets errno], [gl_cv_func_fdopen_works], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include int main (void) { FILE *fp; errno = 0; fp = fdopen (-1, "r"); if (fp == NULL && errno == 0) return 1; return 0; }]])], [gl_cv_func_fdopen_works=yes], [gl_cv_func_fdopen_works=no], [case "$host_os" in mingw*) gl_cv_func_fdopen_works="guessing no" ;; *) gl_cv_func_fdopen_works="guessing yes" ;; esac ]) ]) case "$gl_cv_func_fdopen_works" in *no) REPLACE_FDOPEN=1 ;; esac fi ]) dnl Prerequisites of lib/fdopen.c. AC_DEFUN([gl_PREREQ_FDOPEN], []) gnuastro-0.5/bootstrapped/m4/fcntl_h.m40000644000175000017500000000327113217200022015036 00000000000000# serial 15 # Configure fcntl.h. dnl Copyright (C) 2006-2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. AC_DEFUN([gl_FCNTL_H], [ AC_REQUIRE([gl_FCNTL_H_DEFAULTS]) AC_REQUIRE([gl_FCNTL_O_FLAGS]) gl_NEXT_HEADERS([fcntl.h]) dnl Ensure the type pid_t gets defined. AC_REQUIRE([AC_TYPE_PID_T]) dnl Ensure the type mode_t gets defined. AC_REQUIRE([AC_TYPE_MODE_T]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use, if it is not common dnl enough to be declared everywhere. gl_WARN_ON_USE_PREPARE([[#include ]], [fcntl openat]) ]) AC_DEFUN([gl_FCNTL_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_FCNTL_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) dnl Define it also as a C macro, for the benefit of the unit tests. gl_MODULE_INDICATOR_FOR_TESTS([$1]) ]) AC_DEFUN([gl_FCNTL_H_DEFAULTS], [ GNULIB_FCNTL=0; AC_SUBST([GNULIB_FCNTL]) GNULIB_NONBLOCKING=0; AC_SUBST([GNULIB_NONBLOCKING]) GNULIB_OPEN=0; AC_SUBST([GNULIB_OPEN]) GNULIB_OPENAT=0; AC_SUBST([GNULIB_OPENAT]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_FCNTL=1; AC_SUBST([HAVE_FCNTL]) HAVE_OPENAT=1; AC_SUBST([HAVE_OPENAT]) REPLACE_FCNTL=0; AC_SUBST([REPLACE_FCNTL]) REPLACE_OPEN=0; AC_SUBST([REPLACE_OPEN]) REPLACE_OPENAT=0; AC_SUBST([REPLACE_OPENAT]) ]) gnuastro-0.5/bootstrapped/m4/fcntl.m40000644000175000017500000001035113217200022014524 00000000000000# fcntl.m4 serial 9 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # For now, this module ensures that fcntl() # - supports F_DUPFD correctly # - supports or emulates F_DUPFD_CLOEXEC # - supports F_GETFD # Still to be ported to mingw: # - F_SETFD # - F_GETFL, F_SETFL # - F_GETOWN, F_SETOWN # - F_GETLK, F_SETLK, F_SETLKW AC_DEFUN([gl_FUNC_FCNTL], [ dnl Persuade glibc to expose F_DUPFD_CLOEXEC. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_REQUIRE([gl_FCNTL_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) AC_CHECK_FUNCS_ONCE([fcntl]) if test $ac_cv_func_fcntl = no; then gl_REPLACE_FCNTL else dnl cygwin 1.5.x F_DUPFD has wrong errno, and allows negative target dnl haiku alpha 2 F_DUPFD has wrong errno AC_CACHE_CHECK([whether fcntl handles F_DUPFD correctly], [gl_cv_func_fcntl_f_dupfd_works], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #include #include #include #ifndef RLIM_SAVED_CUR # define RLIM_SAVED_CUR RLIM_INFINITY #endif #ifndef RLIM_SAVED_MAX # define RLIM_SAVED_MAX RLIM_INFINITY #endif ]], [[int result = 0; int bad_fd = INT_MAX; struct rlimit rlim; if (getrlimit (RLIMIT_NOFILE, &rlim) == 0 && 0 <= rlim.rlim_cur && rlim.rlim_cur <= INT_MAX && rlim.rlim_cur != RLIM_INFINITY && rlim.rlim_cur != RLIM_SAVED_MAX && rlim.rlim_cur != RLIM_SAVED_CUR) bad_fd = rlim.rlim_cur; if (fcntl (0, F_DUPFD, -1) != -1) result |= 1; if (errno != EINVAL) result |= 2; if (fcntl (0, F_DUPFD, bad_fd) != -1) result |= 4; if (errno != EINVAL) result |= 8; /* On OS/2 kLIBC, F_DUPFD does not work on a directory fd */ { int fd; fd = open (".", O_RDONLY); if (fd == -1) result |= 16; else if (fcntl (fd, F_DUPFD, STDERR_FILENO + 1) == -1) result |= 32; close (fd); } return result;]])], [gl_cv_func_fcntl_f_dupfd_works=yes], [gl_cv_func_fcntl_f_dupfd_works=no], [case $host_os in aix* | cygwin* | haiku*) gl_cv_func_fcntl_f_dupfd_works="guessing no" ;; *) gl_cv_func_fcntl_f_dupfd_works="guessing yes" ;; esac])]) case $gl_cv_func_fcntl_f_dupfd_works in *yes) ;; *) gl_REPLACE_FCNTL AC_DEFINE([FCNTL_DUPFD_BUGGY], [1], [Define this to 1 if F_DUPFD behavior does not match POSIX]) ;; esac dnl Many systems lack F_DUPFD_CLOEXEC AC_CACHE_CHECK([whether fcntl understands F_DUPFD_CLOEXEC], [gl_cv_func_fcntl_f_dupfd_cloexec], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[ #include #ifndef F_DUPFD_CLOEXEC choke me #endif ]])], [AC_COMPILE_IFELSE([AC_LANG_PROGRAM([[ #ifdef __linux__ /* The Linux kernel only added F_DUPFD_CLOEXEC in 2.6.24, so we always replace it to support the semantics on older kernels that failed with EINVAL. */ choke me #endif ]])], [gl_cv_func_fcntl_f_dupfd_cloexec=yes], [gl_cv_func_fcntl_f_dupfd_cloexec="needs runtime check"])], [gl_cv_func_fcntl_f_dupfd_cloexec=no])]) if test "$gl_cv_func_fcntl_f_dupfd_cloexec" != yes; then gl_REPLACE_FCNTL dnl No witness macro needed for this bug. fi fi dnl Replace fcntl() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then gl_REPLACE_FCNTL fi ]) ]) AC_DEFUN([gl_REPLACE_FCNTL], [ AC_REQUIRE([gl_FCNTL_H_DEFAULTS]) AC_CHECK_FUNCS_ONCE([fcntl]) if test $ac_cv_func_fcntl = no; then HAVE_FCNTL=0 else REPLACE_FCNTL=1 fi ]) gnuastro-0.5/bootstrapped/m4/fcntl-o.m40000644000175000017500000001144013217200022014760 00000000000000# fcntl-o.m4 serial 5 dnl Copyright (C) 2006, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. # Test whether the flags O_NOATIME and O_NOFOLLOW actually work. # Define HAVE_WORKING_O_NOATIME to 1 if O_NOATIME works, or to 0 otherwise. # Define HAVE_WORKING_O_NOFOLLOW to 1 if O_NOFOLLOW works, or to 0 otherwise. AC_DEFUN([gl_FCNTL_O_FLAGS], [ dnl Persuade glibc to define O_NOATIME and O_NOFOLLOW. dnl AC_USE_SYSTEM_EXTENSIONS was introduced in autoconf 2.60 and obsoletes dnl AC_GNU_SOURCE. m4_ifdef([AC_USE_SYSTEM_EXTENSIONS], [AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS])], [AC_REQUIRE([AC_GNU_SOURCE])]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CHECK_HEADERS_ONCE([unistd.h]) AC_CHECK_FUNCS_ONCE([symlink]) AC_CACHE_CHECK([for working fcntl.h], [gl_cv_header_working_fcntl_h], [AC_RUN_IFELSE( [AC_LANG_PROGRAM( [[#include #include #if HAVE_UNISTD_H # include #else /* on Windows with MSVC */ # include # include # defined sleep(n) _sleep ((n) * 1000) #endif #include #ifndef O_NOATIME #define O_NOATIME 0 #endif #ifndef O_NOFOLLOW #define O_NOFOLLOW 0 #endif static int const constants[] = { O_CREAT, O_EXCL, O_NOCTTY, O_TRUNC, O_APPEND, O_NONBLOCK, O_SYNC, O_ACCMODE, O_RDONLY, O_RDWR, O_WRONLY }; ]], [[ int result = !constants; #if HAVE_SYMLINK { static char const sym[] = "conftest.sym"; if (symlink ("/dev/null", sym) != 0) result |= 2; else { int fd = open (sym, O_WRONLY | O_NOFOLLOW | O_CREAT, 0); if (fd >= 0) { close (fd); result |= 4; } } if (unlink (sym) != 0 || symlink (".", sym) != 0) result |= 2; else { int fd = open (sym, O_RDONLY | O_NOFOLLOW); if (fd >= 0) { close (fd); result |= 4; } } unlink (sym); } #endif { static char const file[] = "confdefs.h"; int fd = open (file, O_RDONLY | O_NOATIME); if (fd < 0) result |= 8; else { struct stat st0; if (fstat (fd, &st0) != 0) result |= 16; else { char c; sleep (1); if (read (fd, &c, 1) != 1) result |= 24; else { if (close (fd) != 0) result |= 32; else { struct stat st1; if (stat (file, &st1) != 0) result |= 40; else if (st0.st_atime != st1.st_atime) result |= 64; } } } } } return result;]])], [gl_cv_header_working_fcntl_h=yes], [case $? in #( 4) gl_cv_header_working_fcntl_h='no (bad O_NOFOLLOW)';; #( 64) gl_cv_header_working_fcntl_h='no (bad O_NOATIME)';; #( 68) gl_cv_header_working_fcntl_h='no (bad O_NOATIME, O_NOFOLLOW)';; #( *) gl_cv_header_working_fcntl_h='no';; esac], [case "$host_os" in # Guess 'no' on native Windows. mingw*) gl_cv_header_working_fcntl_h='no' ;; *) gl_cv_header_working_fcntl_h=cross-compiling ;; esac ]) ]) case $gl_cv_header_working_fcntl_h in #( *O_NOATIME* | no | cross-compiling) ac_val=0;; #( *) ac_val=1;; esac AC_DEFINE_UNQUOTED([HAVE_WORKING_O_NOATIME], [$ac_val], [Define to 1 if O_NOATIME works.]) case $gl_cv_header_working_fcntl_h in #( *O_NOFOLLOW* | no | cross-compiling) ac_val=0;; #( *) ac_val=1;; esac AC_DEFINE_UNQUOTED([HAVE_WORKING_O_NOFOLLOW], [$ac_val], [Define to 1 if O_NOFOLLOW works.]) ]) gnuastro-0.5/bootstrapped/m4/extern-inline.m40000644000175000017500000001036313217200022016202 00000000000000dnl 'extern inline' a la ISO C99. dnl Copyright 2012-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_EXTERN_INLINE], [ AH_VERBATIM([extern_inline], [/* Please see the Gnulib manual for how to use these macros. Suppress extern inline with HP-UX cc, as it appears to be broken; see . Suppress extern inline with Sun C in standards-conformance mode, as it mishandles inline functions that call each other. E.g., for 'inline void f (void) { } inline void g (void) { f (); }', c99 incorrectly complains 'reference to static identifier "f" in extern inline function'. This bug was observed with Sun C 5.12 SunOS_i386 2011/11/16. Suppress extern inline (with or without __attribute__ ((__gnu_inline__))) on configurations that mistakenly use 'static inline' to implement functions or macros in standard C headers like . For example, if isdigit is mistakenly implemented via a static inline function, a program containing an extern inline function that calls isdigit may not work since the C standard prohibits extern inline functions from calling static functions. This bug is known to occur on: OS X 10.8 and earlier; see: https://lists.gnu.org/r/bug-gnulib/2012-12/msg00023.html DragonFly; see http://muscles.dragonflybsd.org/bulk/bleeding-edge-potential/latest-per-pkg/ah-tty-0.3.12.log FreeBSD; see: https://lists.gnu.org/r/bug-gnulib/2014-07/msg00104.html OS X 10.9 has a macro __header_inline indicating the bug is fixed for C and for clang but remains for g++; see . Assume DragonFly and FreeBSD will be similar. */ #if (((defined __APPLE__ && defined __MACH__) \ || defined __DragonFly__ || defined __FreeBSD__) \ && (defined __header_inline \ ? (defined __cplusplus && defined __GNUC_STDC_INLINE__ \ && ! defined __clang__) \ : ((! defined _DONT_USE_CTYPE_INLINE_ \ && (defined __GNUC__ || defined __cplusplus)) \ || (defined _FORTIFY_SOURCE && 0 < _FORTIFY_SOURCE \ && defined __GNUC__ && ! defined __cplusplus)))) # define _GL_EXTERN_INLINE_STDHEADER_BUG #endif #if ((__GNUC__ \ ? defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ \ : (199901L <= __STDC_VERSION__ \ && !defined __HP_cc \ && !defined __PGI \ && !(defined __SUNPRO_C && __STDC__))) \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # define _GL_INLINE inline # define _GL_EXTERN_INLINE extern inline # define _GL_EXTERN_INLINE_IN_USE #elif (2 < __GNUC__ + (7 <= __GNUC_MINOR__) && !defined __STRICT_ANSI__ \ && !defined _GL_EXTERN_INLINE_STDHEADER_BUG) # if defined __GNUC_GNU_INLINE__ && __GNUC_GNU_INLINE__ /* __gnu_inline__ suppresses a GCC 4.2 diagnostic. */ # define _GL_INLINE extern inline __attribute__ ((__gnu_inline__)) # else # define _GL_INLINE extern inline # endif # define _GL_EXTERN_INLINE extern # define _GL_EXTERN_INLINE_IN_USE #else # define _GL_INLINE static _GL_UNUSED # define _GL_EXTERN_INLINE static _GL_UNUSED #endif /* In GCC 4.6 (inclusive) to 5.1 (exclusive), suppress bogus "no previous prototype for 'FOO'" and "no previous declaration for 'FOO'" diagnostics, when FOO is an inline function in the header; see and . */ #if __GNUC__ == 4 && 6 <= __GNUC_MINOR__ # if defined __GNUC_STDC_INLINE__ && __GNUC_STDC_INLINE__ # define _GL_INLINE_HEADER_CONST_PRAGMA # else # define _GL_INLINE_HEADER_CONST_PRAGMA \ _Pragma ("GCC diagnostic ignored \"-Wsuggest-attribute=const\"") # endif # define _GL_INLINE_HEADER_BEGIN \ _Pragma ("GCC diagnostic push") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-prototypes\"") \ _Pragma ("GCC diagnostic ignored \"-Wmissing-declarations\"") \ _GL_INLINE_HEADER_CONST_PRAGMA # define _GL_INLINE_HEADER_END \ _Pragma ("GCC diagnostic pop") #else # define _GL_INLINE_HEADER_BEGIN # define _GL_INLINE_HEADER_END #endif]) ]) gnuastro-0.5/bootstrapped/m4/extensions.m40000644000175000017500000001536513217200022015627 00000000000000# serial 17 -*- Autoconf -*- # Enable extensions on systems that normally disable them. # Copyright (C) 2003, 2006-2017 Free Software Foundation, Inc. # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This definition of AC_USE_SYSTEM_EXTENSIONS is stolen from git # Autoconf. Perhaps we can remove this once we can assume Autoconf # 2.70 or later everywhere, but since Autoconf mutates rapidly # enough in this area it's likely we'll need to redefine # AC_USE_SYSTEM_EXTENSIONS for quite some time. # If autoconf reports a warning # warning: AC_COMPILE_IFELSE was called before AC_USE_SYSTEM_EXTENSIONS # or warning: AC_RUN_IFELSE was called before AC_USE_SYSTEM_EXTENSIONS # the fix is # 1) to ensure that AC_USE_SYSTEM_EXTENSIONS is never directly invoked # but always AC_REQUIREd, # 2) to ensure that for each occurrence of # AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) # or # AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) # the corresponding gnulib module description has 'extensions' among # its dependencies. This will ensure that the gl_USE_SYSTEM_EXTENSIONS # invocation occurs in gl_EARLY, not in gl_INIT. # AC_USE_SYSTEM_EXTENSIONS # ------------------------ # Enable extensions on systems that normally disable them, # typically due to standards-conformance issues. # # Remember that #undef in AH_VERBATIM gets replaced with #define by # AC_DEFINE. The goal here is to define all known feature-enabling # macros, then, if reports of conflicts are made, disable macros that # cause problems on some platforms (such as __EXTENSIONS__). AC_DEFUN_ONCE([AC_USE_SYSTEM_EXTENSIONS], [AC_BEFORE([$0], [AC_COMPILE_IFELSE])dnl AC_BEFORE([$0], [AC_RUN_IFELSE])dnl AC_CHECK_HEADER([minix/config.h], [MINIX=yes], [MINIX=]) if test "$MINIX" = yes; then AC_DEFINE([_POSIX_SOURCE], [1], [Define to 1 if you need to in order for 'stat' and other things to work.]) AC_DEFINE([_POSIX_1_SOURCE], [2], [Define to 2 if the system does not provide POSIX.1 features except with this defined.]) AC_DEFINE([_MINIX], [1], [Define to 1 if on MINIX.]) AC_DEFINE([_NETBSD_SOURCE], [1], [Define to 1 to make NetBSD features available. MINIX 3 needs this.]) fi dnl Use a different key than __EXTENSIONS__, as that name broke existing dnl configure.ac when using autoheader 2.62. AH_VERBATIM([USE_SYSTEM_EXTENSIONS], [/* Enable extensions on AIX 3, Interix. */ #ifndef _ALL_SOURCE # undef _ALL_SOURCE #endif /* Enable general extensions on macOS. */ #ifndef _DARWIN_C_SOURCE # undef _DARWIN_C_SOURCE #endif /* Enable GNU extensions on systems that have them. */ #ifndef _GNU_SOURCE # undef _GNU_SOURCE #endif /* Enable NetBSD extensions on NetBSD. */ #ifndef _NETBSD_SOURCE # undef _NETBSD_SOURCE #endif /* Enable OpenBSD extensions on NetBSD. */ #ifndef _OPENBSD_SOURCE # undef _OPENBSD_SOURCE #endif /* Enable threading extensions on Solaris. */ #ifndef _POSIX_PTHREAD_SEMANTICS # undef _POSIX_PTHREAD_SEMANTICS #endif /* Enable extensions specified by ISO/IEC TS 18661-5:2014. */ #ifndef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ # undef __STDC_WANT_IEC_60559_ATTRIBS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-1:2014. */ #ifndef __STDC_WANT_IEC_60559_BFP_EXT__ # undef __STDC_WANT_IEC_60559_BFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-2:2015. */ #ifndef __STDC_WANT_IEC_60559_DFP_EXT__ # undef __STDC_WANT_IEC_60559_DFP_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-4:2015. */ #ifndef __STDC_WANT_IEC_60559_FUNCS_EXT__ # undef __STDC_WANT_IEC_60559_FUNCS_EXT__ #endif /* Enable extensions specified by ISO/IEC TS 18661-3:2015. */ #ifndef __STDC_WANT_IEC_60559_TYPES_EXT__ # undef __STDC_WANT_IEC_60559_TYPES_EXT__ #endif /* Enable extensions specified by ISO/IEC TR 24731-2:2010. */ #ifndef __STDC_WANT_LIB_EXT2__ # undef __STDC_WANT_LIB_EXT2__ #endif /* Enable extensions specified by ISO/IEC 24747:2009. */ #ifndef __STDC_WANT_MATH_SPEC_FUNCS__ # undef __STDC_WANT_MATH_SPEC_FUNCS__ #endif /* Enable extensions on HP NonStop. */ #ifndef _TANDEM_SOURCE # undef _TANDEM_SOURCE #endif /* Enable X/Open extensions if necessary. HP-UX 11.11 defines mbstate_t only if _XOPEN_SOURCE is defined to 500, regardless of whether compiling with -Ae or -D_HPUX_SOURCE=1. */ #ifndef _XOPEN_SOURCE # undef _XOPEN_SOURCE #endif /* Enable general extensions on Solaris. */ #ifndef __EXTENSIONS__ # undef __EXTENSIONS__ #endif ]) AC_CACHE_CHECK([whether it is safe to define __EXTENSIONS__], [ac_cv_safe_to_define___extensions__], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ # define __EXTENSIONS__ 1 ]AC_INCLUDES_DEFAULT])], [ac_cv_safe_to_define___extensions__=yes], [ac_cv_safe_to_define___extensions__=no])]) test $ac_cv_safe_to_define___extensions__ = yes && AC_DEFINE([__EXTENSIONS__]) AC_DEFINE([_ALL_SOURCE]) AC_DEFINE([_DARWIN_C_SOURCE]) AC_DEFINE([_GNU_SOURCE]) AC_DEFINE([_NETBSD_SOURCE]) AC_DEFINE([_OPENBSD_SOURCE]) AC_DEFINE([_POSIX_PTHREAD_SEMANTICS]) AC_DEFINE([__STDC_WANT_IEC_60559_ATTRIBS_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_BFP_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_DFP_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_FUNCS_EXT__]) AC_DEFINE([__STDC_WANT_IEC_60559_TYPES_EXT__]) AC_DEFINE([__STDC_WANT_LIB_EXT2__]) AC_DEFINE([__STDC_WANT_MATH_SPEC_FUNCS__]) AC_DEFINE([_TANDEM_SOURCE]) AC_CACHE_CHECK([whether _XOPEN_SOURCE should be defined], [ac_cv_should_define__xopen_source], [ac_cv_should_define__xopen_source=no AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ #include mbstate_t x;]])], [], [AC_COMPILE_IFELSE( [AC_LANG_PROGRAM([[ #define _XOPEN_SOURCE 500 #include mbstate_t x;]])], [ac_cv_should_define__xopen_source=yes])])]) test $ac_cv_should_define__xopen_source = yes && AC_DEFINE([_XOPEN_SOURCE], [500]) ])# AC_USE_SYSTEM_EXTENSIONS # gl_USE_SYSTEM_EXTENSIONS # ------------------------ # Enable extensions on systems that normally disable them, # typically due to standards-conformance issues. AC_DEFUN_ONCE([gl_USE_SYSTEM_EXTENSIONS], [ dnl Require this macro before AC_USE_SYSTEM_EXTENSIONS. dnl gnulib does not need it. But if it gets required by third-party macros dnl after AC_USE_SYSTEM_EXTENSIONS is required, autoconf 2.62..2.63 emit a dnl warning: "AC_COMPILE_IFELSE was called before AC_USE_SYSTEM_EXTENSIONS". dnl Note: We can do this only for one of the macros AC_AIX, AC_GNU_SOURCE, dnl AC_MINIX. If people still use AC_AIX or AC_MINIX, they are out of luck. AC_REQUIRE([AC_GNU_SOURCE]) AC_REQUIRE([AC_USE_SYSTEM_EXTENSIONS]) ]) gnuastro-0.5/bootstrapped/m4/exponentl.m40000644000175000017500000000713713217200022015442 00000000000000# exponentl.m4 serial 4 dnl Copyright (C) 2007-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_LONG_DOUBLE_EXPONENT_LOCATION], [ AC_REQUIRE([gl_BIGENDIAN]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles AC_CACHE_CHECK([where to find the exponent in a 'long double'], [gl_cv_cc_long_double_expbit0], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #define NWORDS \ ((sizeof (long double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { long double value; unsigned int word[NWORDS]; } memory_long_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (long double x) { memory_long_double m; size_t i; /* Clear it first, in case sizeof (long double) < sizeof (memory_long_double). */ memset (&m, 0, sizeof (memory_long_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25L); add_to_ored_words (0.5L); add_to_ored_words (1.0L); add_to_ored_words (2.0L); add_to_ored_words (4.0L); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } ]])], [gl_cv_cc_long_double_expbit0=`cat conftest.out`], [gl_cv_cc_long_double_expbit0="unknown"], [ dnl When cross-compiling, in general we don't know. It depends on the dnl ABI and compiler version. There are too many cases. gl_cv_cc_long_double_expbit0="unknown" case "$host_os" in mingw*) # On native Windows (little-endian), we know the result # in two cases: mingw, MSVC. AC_EGREP_CPP([Known], [ #ifdef __MINGW32__ Known #endif ], [gl_cv_cc_long_double_expbit0="word 2 bit 0"]) AC_EGREP_CPP([Known], [ #ifdef _MSC_VER Known #endif ], [gl_cv_cc_long_double_expbit0="word 1 bit 20"]) ;; esac ]) rm -f conftest.out ]) case "$gl_cv_cc_long_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_long_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_long_double_expbit0" | sed -e 's/word.*bit //'` AC_DEFINE_UNQUOTED([LDBL_EXPBIT0_WORD], [$word], [Define as the word index where to find the exponent of 'long double'.]) AC_DEFINE_UNQUOTED([LDBL_EXPBIT0_BIT], [$bit], [Define as the bit index in the word where to find bit 0 of the exponent of 'long double'.]) ;; esac ]) gnuastro-0.5/bootstrapped/m4/exponentf.m40000644000175000017500000000545613217200022015436 00000000000000# exponentf.m4 serial 2 dnl Copyright (C) 2007-2008, 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FLOAT_EXPONENT_LOCATION], [ AC_CACHE_CHECK([where to find the exponent in a 'float'], [gl_cv_cc_float_expbit0], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #define NWORDS \ ((sizeof (float) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { float value; unsigned int word[NWORDS]; } memory_float; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (float x) { memory_float m; size_t i; /* Clear it first, in case sizeof (float) < sizeof (memory_float). */ memset (&m, 0, sizeof (memory_float)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25f); add_to_ored_words (0.5f); add_to_ored_words (1.0f); add_to_ored_words (2.0f); add_to_ored_words (4.0f); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } ]])], [gl_cv_cc_float_expbit0=`cat conftest.out`], [gl_cv_cc_float_expbit0="unknown"], [gl_cv_cc_float_expbit0="word 0 bit 23"]) rm -f conftest.out ]) case "$gl_cv_cc_float_expbit0" in word*bit*) word=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_float_expbit0" | sed -e 's/word.*bit //'` AC_DEFINE_UNQUOTED([FLT_EXPBIT0_WORD], [$word], [Define as the word index where to find the exponent of 'float'.]) AC_DEFINE_UNQUOTED([FLT_EXPBIT0_BIT], [$bit], [Define as the bit index in the word where to find bit 0 of the exponent of 'float'.]) ;; esac ]) gnuastro-0.5/bootstrapped/m4/exponentd.m40000644000175000017500000000755213217200022015433 00000000000000# exponentd.m4 serial 3 dnl Copyright (C) 2007-2008, 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_DOUBLE_EXPONENT_LOCATION], [ AC_CACHE_CHECK([where to find the exponent in a 'double'], [gl_cv_cc_double_expbit0], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include #include #include #define NWORDS \ ((sizeof (double) + sizeof (unsigned int) - 1) / sizeof (unsigned int)) typedef union { double value; unsigned int word[NWORDS]; } memory_double; static unsigned int ored_words[NWORDS]; static unsigned int anded_words[NWORDS]; static void add_to_ored_words (double x) { memory_double m; size_t i; /* Clear it first, in case sizeof (double) < sizeof (memory_double). */ memset (&m, 0, sizeof (memory_double)); m.value = x; for (i = 0; i < NWORDS; i++) { ored_words[i] |= m.word[i]; anded_words[i] &= m.word[i]; } } int main () { size_t j; FILE *fp = fopen ("conftest.out", "w"); if (fp == NULL) return 1; for (j = 0; j < NWORDS; j++) anded_words[j] = ~ (unsigned int) 0; add_to_ored_words (0.25); add_to_ored_words (0.5); add_to_ored_words (1.0); add_to_ored_words (2.0); add_to_ored_words (4.0); /* Remove bits that are common (e.g. if representation of the first mantissa bit is explicit). */ for (j = 0; j < NWORDS; j++) ored_words[j] &= ~anded_words[j]; /* Now find the nonzero word. */ for (j = 0; j < NWORDS; j++) if (ored_words[j] != 0) break; if (j < NWORDS) { size_t i; for (i = j + 1; i < NWORDS; i++) if (ored_words[i] != 0) { fprintf (fp, "unknown"); return (fclose (fp) != 0); } for (i = 0; ; i++) if ((ored_words[j] >> i) & 1) { fprintf (fp, "word %d bit %d", (int) j, (int) i); return (fclose (fp) != 0); } } fprintf (fp, "unknown"); return (fclose (fp) != 0); } ]])], [gl_cv_cc_double_expbit0=`cat conftest.out`], [gl_cv_cc_double_expbit0="unknown"], [ dnl On ARM, there are two 'double' floating-point formats, used by dnl different sets of instructions: The older FPA instructions assume dnl that they are stored in big-endian word order, while the words dnl (like integer types) are stored in little-endian byte order. dnl The newer VFP instructions assume little-endian order dnl consistently. AC_EGREP_CPP([mixed_endianness], [ #if defined arm || defined __arm || defined __arm__ mixed_endianness #endif ], [gl_cv_cc_double_expbit0="unknown"], [ pushdef([AC_MSG_CHECKING],[:])dnl pushdef([AC_MSG_RESULT],[:])dnl pushdef([AC_MSG_RESULT_UNQUOTED],[:])dnl AC_C_BIGENDIAN( [gl_cv_cc_double_expbit0="word 0 bit 20"], [gl_cv_cc_double_expbit0="word 1 bit 20"], [gl_cv_cc_double_expbit0="unknown"]) popdef([AC_MSG_RESULT_UNQUOTED])dnl popdef([AC_MSG_RESULT])dnl popdef([AC_MSG_CHECKING])dnl ]) ]) rm -f conftest.out ]) case "$gl_cv_cc_double_expbit0" in word*bit*) word=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word //' -e 's/ bit.*//'` bit=`echo "$gl_cv_cc_double_expbit0" | sed -e 's/word.*bit //'` AC_DEFINE_UNQUOTED([DBL_EXPBIT0_WORD], [$word], [Define as the word index where to find the exponent of 'double'.]) AC_DEFINE_UNQUOTED([DBL_EXPBIT0_BIT], [$bit], [Define as the bit index in the word where to find bit 0 of the exponent of 'double'.]) ;; esac ]) gnuastro-0.5/bootstrapped/m4/error.m40000644000175000017500000000151013217200022014544 00000000000000#serial 14 # Copyright (C) 1996-1998, 2001-2004, 2009-2017 Free Software Foundation, Inc. # # This file is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_ERROR], [ dnl We don't use AC_FUNC_ERROR_AT_LINE any more, because it is no longer dnl maintained in Autoconf and because it invokes AC_LIBOBJ. AC_CACHE_CHECK([for error_at_line], [ac_cv_lib_error_at_line], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[error_at_line (0, 0, "", 0, "an error occurred");]])], [ac_cv_lib_error_at_line=yes], [ac_cv_lib_error_at_line=no])]) ]) # Prerequisites of lib/error.c. AC_DEFUN([gl_PREREQ_ERROR], [ AC_REQUIRE([AC_FUNC_STRERROR_R]) : ]) gnuastro-0.5/bootstrapped/m4/errno_h.m40000644000175000017500000000623413217200022015057 00000000000000# errno_h.m4 serial 12 dnl Copyright (C) 2004, 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_HEADER_ERRNO_H], [ AC_REQUIRE([AC_PROG_CC]) AC_CACHE_CHECK([for complete errno.h], [gl_cv_header_errno_h_complete], [ AC_EGREP_CPP([booboo],[ #include #if !defined ETXTBSY booboo #endif #if !defined ENOMSG booboo #endif #if !defined EIDRM booboo #endif #if !defined ENOLINK booboo #endif #if !defined EPROTO booboo #endif #if !defined EMULTIHOP booboo #endif #if !defined EBADMSG booboo #endif #if !defined EOVERFLOW booboo #endif #if !defined ENOTSUP booboo #endif #if !defined ENETRESET booboo #endif #if !defined ECONNABORTED booboo #endif #if !defined ESTALE booboo #endif #if !defined EDQUOT booboo #endif #if !defined ECANCELED booboo #endif #if !defined EOWNERDEAD booboo #endif #if !defined ENOTRECOVERABLE booboo #endif #if !defined EILSEQ booboo #endif ], [gl_cv_header_errno_h_complete=no], [gl_cv_header_errno_h_complete=yes]) ]) if test $gl_cv_header_errno_h_complete = yes; then ERRNO_H='' else gl_NEXT_HEADERS([errno.h]) ERRNO_H='errno.h' fi AC_SUBST([ERRNO_H]) AM_CONDITIONAL([GL_GENERATE_ERRNO_H], [test -n "$ERRNO_H"]) gl_REPLACE_ERRNO_VALUE([EMULTIHOP]) gl_REPLACE_ERRNO_VALUE([ENOLINK]) gl_REPLACE_ERRNO_VALUE([EOVERFLOW]) ]) # Assuming $1 = EOVERFLOW. # The EOVERFLOW errno value ought to be defined in , according to # POSIX. But some systems (like OpenBSD 4.0 or AIX 3) don't define it, and # some systems (like OSF/1) define it when _XOPEN_SOURCE_EXTENDED is defined. # Check for the value of EOVERFLOW. # Set the variables EOVERFLOW_HIDDEN and EOVERFLOW_VALUE. AC_DEFUN([gl_REPLACE_ERRNO_VALUE], [ if test -n "$ERRNO_H"; then AC_CACHE_CHECK([for ]$1[ value], [gl_cv_header_errno_h_]$1, [ AC_EGREP_CPP([yes],[ #include #ifdef ]$1[ yes #endif ], [gl_cv_header_errno_h_]$1[=yes], [gl_cv_header_errno_h_]$1[=no]) if test $gl_cv_header_errno_h_]$1[ = no; then AC_EGREP_CPP([yes],[ #define _XOPEN_SOURCE_EXTENDED 1 #include #ifdef ]$1[ yes #endif ], [gl_cv_header_errno_h_]$1[=hidden]) if test $gl_cv_header_errno_h_]$1[ = hidden; then dnl The macro exists but is hidden. dnl Define it to the same value. AC_COMPUTE_INT([gl_cv_header_errno_h_]$1, $1, [ #define _XOPEN_SOURCE_EXTENDED 1 #include /* The following two lines are a workaround against an autoconf-2.52 bug. */ #include #include ]) fi fi ]) case $gl_cv_header_errno_h_]$1[ in yes | no) ]$1[_HIDDEN=0; ]$1[_VALUE= ;; *) ]$1[_HIDDEN=1; ]$1[_VALUE="$gl_cv_header_errno_h_]$1[" ;; esac AC_SUBST($1[_HIDDEN]) AC_SUBST($1[_VALUE]) fi ]) dnl Autoconf >= 2.61 has AC_COMPUTE_INT built-in. dnl Remove this when we can assume autoconf >= 2.61. m4_ifdef([AC_COMPUTE_INT], [], [ AC_DEFUN([AC_COMPUTE_INT], [_AC_COMPUTE_INT([$2],[$1],[$3],[$4])]) ]) gnuastro-0.5/bootstrapped/m4/environ.m40000644000175000017500000000261613217200022015103 00000000000000# environ.m4 serial 6 dnl Copyright (C) 2001-2004, 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN_ONCE([gl_ENVIRON], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) dnl Persuade glibc to declare environ. AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_HEADERS_ONCE([unistd.h]) gt_CHECK_VAR_DECL( [#if HAVE_UNISTD_H #include #endif /* mingw, BeOS, Haiku declare environ in , not in . */ #include ], [environ]) if test $gt_cv_var_environ_declaration != yes; then HAVE_DECL_ENVIRON=0 fi ]) # Check if a variable is properly declared. # gt_CHECK_VAR_DECL(includes,variable) AC_DEFUN([gt_CHECK_VAR_DECL], [ define([gt_cv_var], [gt_cv_var_]$2[_declaration]) AC_MSG_CHECKING([if $2 is properly declared]) AC_CACHE_VAL([gt_cv_var], [ AC_COMPILE_IFELSE( [AC_LANG_PROGRAM( [[$1 extern struct { int foo; } $2;]], [[$2.foo = 1;]])], [gt_cv_var=no], [gt_cv_var=yes])]) AC_MSG_RESULT([$gt_cv_var]) if test $gt_cv_var = yes; then AC_DEFINE([HAVE_]m4_translit($2, [a-z], [A-Z])[_DECL], 1, [Define if you have the declaration of $2.]) fi undefine([gt_cv_var]) ]) gnuastro-0.5/bootstrapped/m4/eealloc.m40000644000175000017500000000166713217200022015034 00000000000000# eealloc.m4 serial 3 dnl Copyright (C) 2003, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_EEALLOC], [ AC_REQUIRE([gl_EEMALLOC]) AC_REQUIRE([gl_EEREALLOC]) ]) AC_DEFUN([gl_EEMALLOC], [ _AC_FUNC_MALLOC_IF( [gl_cv_func_malloc_0_nonnull=1], [gl_cv_func_malloc_0_nonnull=0]) AC_DEFINE_UNQUOTED([MALLOC_0_IS_NONNULL], [$gl_cv_func_malloc_0_nonnull], [If malloc(0) is != NULL, define this to 1. Otherwise define this to 0.]) ]) AC_DEFUN([gl_EEREALLOC], [ _AC_FUNC_REALLOC_IF( [gl_cv_func_realloc_0_nonnull=1], [gl_cv_func_realloc_0_nonnull=0]) AC_DEFINE_UNQUOTED([REALLOC_0_IS_NONNULL], [$gl_cv_func_realloc_0_nonnull], [If realloc(NULL,0) is != NULL, define this to 1. Otherwise define this to 0.]) ]) gnuastro-0.5/bootstrapped/m4/dup2.m40000644000175000017500000001013413217200022014267 00000000000000#serial 25 dnl Copyright (C) 2002, 2005, 2007, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_DUP2], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) AC_REQUIRE([AC_CANONICAL_HOST]) m4_ifdef([gl_FUNC_DUP2_OBSOLETE], [ AC_CHECK_FUNCS_ONCE([dup2]) if test $ac_cv_func_dup2 = no; then HAVE_DUP2=0 fi ], [ AC_DEFINE([HAVE_DUP2], [1], [Define to 1 if you have the 'dup2' function.]) ]) if test $HAVE_DUP2 = 1; then AC_CACHE_CHECK([whether dup2 works], [gl_cv_func_dup2_works], [AC_RUN_IFELSE([ AC_LANG_PROGRAM( [[#include #include #include #include #include #ifndef RLIM_SAVED_CUR # define RLIM_SAVED_CUR RLIM_INFINITY #endif #ifndef RLIM_SAVED_MAX # define RLIM_SAVED_MAX RLIM_INFINITY #endif ]], [[int result = 0; int bad_fd = INT_MAX; struct rlimit rlim; if (getrlimit (RLIMIT_NOFILE, &rlim) == 0 && 0 <= rlim.rlim_cur && rlim.rlim_cur <= INT_MAX && rlim.rlim_cur != RLIM_INFINITY && rlim.rlim_cur != RLIM_SAVED_MAX && rlim.rlim_cur != RLIM_SAVED_CUR) bad_fd = rlim.rlim_cur; #ifdef FD_CLOEXEC if (fcntl (1, F_SETFD, FD_CLOEXEC) == -1) result |= 1; #endif if (dup2 (1, 1) != 1) result |= 2; #ifdef FD_CLOEXEC if (fcntl (1, F_GETFD) != FD_CLOEXEC) result |= 4; #endif close (0); if (dup2 (0, 0) != -1) result |= 8; /* Many gnulib modules require POSIX conformance of EBADF. */ if (dup2 (2, bad_fd) == -1 && errno != EBADF) result |= 16; /* Flush out some cygwin core dumps. */ if (dup2 (2, -1) != -1 || errno != EBADF) result |= 32; dup2 (2, 255); dup2 (2, 256); /* On OS/2 kLIBC, dup2() does not work on a directory fd. */ { int fd = open (".", O_RDONLY); if (fd == -1) result |= 64; else if (dup2 (fd, fd + 1) == -1) result |= 128; close (fd); } return result;]]) ], [gl_cv_func_dup2_works=yes], [gl_cv_func_dup2_works=no], [case "$host_os" in mingw*) # on this platform, dup2 always returns 0 for success gl_cv_func_dup2_works="guessing no" ;; cygwin*) # on cygwin 1.5.x, dup2(1,1) returns 0 gl_cv_func_dup2_works="guessing no" ;; aix* | freebsd*) # on AIX 7.1 and FreeBSD 6.1, dup2 (1,toobig) gives EMFILE, # not EBADF. gl_cv_func_dup2_works="guessing no" ;; haiku*) # on Haiku alpha 2, dup2(1, 1) resets FD_CLOEXEC. gl_cv_func_dup2_works="guessing no" ;; *-android*) # implemented using dup3(), which fails if oldfd == newfd gl_cv_func_dup2_works="guessing no" ;; os2*) # on OS/2 kLIBC, dup2() does not work on a directory fd. gl_cv_func_dup2_works="guessing no" ;; *) gl_cv_func_dup2_works="guessing yes" ;; esac]) ]) case "$gl_cv_func_dup2_works" in *yes) ;; *) REPLACE_DUP2=1 AC_CHECK_FUNCS([setdtablesize]) ;; esac fi dnl Replace dup2() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then if test $HAVE_DUP2 = 1; then REPLACE_DUP2=1 fi fi ]) ]) # Prerequisites of lib/dup2.c. AC_DEFUN([gl_PREREQ_DUP2], []) gnuastro-0.5/bootstrapped/m4/double-slash-root.m40000644000175000017500000000312513217200022016762 00000000000000# double-slash-root.m4 serial 4 -*- Autoconf -*- dnl Copyright (C) 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_DOUBLE_SLASH_ROOT], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_CACHE_CHECK([whether // is distinct from /], [gl_cv_double_slash_root], [ if test x"$cross_compiling" = xyes ; then # When cross-compiling, there is no way to tell whether // is special # short of a list of hosts. However, the only known hosts to date # that have a distinct // are Apollo DomainOS (too old to port to), # Cygwin, and z/OS. If anyone knows of another system for which // has # special semantics and is distinct from /, please report it to # . case $host in *-cygwin | i370-ibm-openedition) gl_cv_double_slash_root=yes ;; *) # Be optimistic and assume that / and // are the same when we # don't know. gl_cv_double_slash_root='unknown, assuming no' ;; esac else set x `ls -di / // 2>/dev/null` if test "$[2]" = "$[4]" && wc //dev/null >/dev/null 2>&1; then gl_cv_double_slash_root=no else gl_cv_double_slash_root=yes fi fi]) if test "$gl_cv_double_slash_root" = yes; then AC_DEFINE([DOUBLE_SLASH_IS_DISTINCT_ROOT], [1], [Define to 1 if // is a file system root distinct from /.]) fi ]) gnuastro-0.5/bootstrapped/m4/dirname.m40000644000175000017500000000105413217200022015035 00000000000000#serial 10 -*- autoconf -*- dnl Copyright (C) 2002-2006, 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_DIRNAME], [ AC_REQUIRE([gl_DIRNAME_LGPL]) ]) AC_DEFUN([gl_DIRNAME_LGPL], [ dnl Prerequisites of lib/dirname.h. AC_REQUIRE([gl_DOUBLE_SLASH_ROOT]) dnl No prerequisites of lib/basename-lgpl.c, lib/dirname-lgpl.c, dnl lib/stripslash.c. ]) gnuastro-0.5/bootstrapped/m4/ctype.m40000644000175000017500000000177513217200022014554 00000000000000# ctype_h.m4 serial 6 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_CTYPE_H], [ AC_REQUIRE([gl_CTYPE_H_DEFAULTS]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_NEXT_HEADERS([ctype.h]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[#include ]], [isblank]) ]) AC_DEFUN([gl_CTYPE_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_CTYPE_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_CTYPE_H_DEFAULTS], [ GNULIB_ISBLANK=0; AC_SUBST([GNULIB_ISBLANK]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_ISBLANK=1; AC_SUBST([HAVE_ISBLANK]) ]) gnuastro-0.5/bootstrapped/m4/configmake.m40000644000175000017500000000402113217200022015516 00000000000000# configmake.m4 serial 2 dnl Copyright (C) 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. # gl_CONFIGMAKE_PREP # ------------------ # Guarantee all of the standard directory variables, even when used with # autoconf 2.59 (datarootdir wasn't supported until 2.59c, and runstatedir # in 2.70) or automake 1.9.6 (pkglibexecdir wasn't supported until 1.10b, # and runstatedir in 1.14.1). AC_DEFUN([gl_CONFIGMAKE_PREP], [ dnl Technically, datadir should default to datarootdir. But if dnl autoconf is too old to provide datarootdir, then reversing the dnl definition is a reasonable compromise. Only AC_SUBST a variable dnl if it was not already defined earlier by autoconf. if test "x$datarootdir" = x; then AC_SUBST([datarootdir], ['${datadir}']) fi dnl Copy the approach used in autoconf 2.60. if test "x$docdir" = x; then AC_SUBST([docdir], [m4_ifset([AC_PACKAGE_TARNAME], ['${datarootdir}/doc/${PACKAGE_TARNAME}'], ['${datarootdir}/doc/${PACKAGE}'])]) fi dnl The remaining variables missing from autoconf 2.59 are easier. if test "x$htmldir" = x; then AC_SUBST([htmldir], ['${docdir}']) fi if test "x$dvidir" = x; then AC_SUBST([dvidir], ['${docdir}']) fi if test "x$pdfdir" = x; then AC_SUBST([pdfdir], ['${docdir}']) fi if test "x$psdir" = x; then AC_SUBST([psdir], ['${docdir}']) fi if test "x$lispdir" = x; then AC_SUBST([lispdir], ['${datarootdir}/emacs/site-lisp']) fi if test "x$localedir" = x; then AC_SUBST([localedir], ['${datarootdir}/locale']) fi dnl Added in autoconf 2.70 if test "x$runstatedir" = x; then AC_SUBST([runstatedir], ['${localstatedir}/run']) fi dnl Automake 1.9.6 only lacks pkglibexecdir; and since 1.11 merely dnl provides it without AC_SUBST, this blind use of AC_SUBST is safe. AC_SUBST([pkglibexecdir], ['${libexecdir}/${PACKAGE}']) ]) gnuastro-0.5/bootstrapped/m4/codeset.m40000644000175000017500000000151213217200022015043 00000000000000# codeset.m4 serial 5 (gettext-0.18.2) dnl Copyright (C) 2000-2002, 2006, 2008-2014, 2016 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. AC_DEFUN([AM_LANGINFO_CODESET], [ AC_CACHE_CHECK([for nl_langinfo and CODESET], [am_cv_langinfo_codeset], [AC_LINK_IFELSE( [AC_LANG_PROGRAM( [[#include ]], [[char* cs = nl_langinfo(CODESET); return !cs;]])], [am_cv_langinfo_codeset=yes], [am_cv_langinfo_codeset=no]) ]) if test $am_cv_langinfo_codeset = yes; then AC_DEFINE([HAVE_LANGINFO_CODESET], [1], [Define if you have and nl_langinfo(CODESET).]) fi ]) gnuastro-0.5/bootstrapped/m4/close.m40000644000175000017500000000222113217200022014520 00000000000000# close.m4 serial 9 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_CLOSE], [ AC_REQUIRE([gl_UNISTD_H_DEFAULTS]) m4_ifdef([gl_MSVC_INVAL], [ AC_REQUIRE([gl_MSVC_INVAL]) if test $HAVE_MSVC_INVALID_PARAMETER_HANDLER = 1; then REPLACE_CLOSE=1 fi ]) m4_ifdef([gl_PREREQ_SYS_H_WINSOCK2], [ gl_PREREQ_SYS_H_WINSOCK2 if test $UNISTD_H_HAVE_WINSOCK2_H = 1; then dnl Even if the 'socket' module is not used here, another part of the dnl application may use it and pass file descriptors that refer to dnl sockets to the close() function. So enable the support for sockets. REPLACE_CLOSE=1 fi ]) dnl Replace close() for supporting the gnulib-defined fchdir() function, dnl to keep fchdir's bookkeeping up-to-date. m4_ifdef([gl_FUNC_FCHDIR], [ if test $REPLACE_CLOSE = 0; then gl_TEST_FCHDIR if test $HAVE_FCHDIR = 0; then REPLACE_CLOSE=1 fi fi ]) ]) gnuastro-0.5/bootstrapped/m4/builtin-expect.m40000644000175000017500000000302313217200022016350 00000000000000dnl Check for __builtin_expect. dnl Copyright 2016-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Paul Eggert. AC_DEFUN([gl___BUILTIN_EXPECT], [ AC_CACHE_CHECK([for __builtin_expect], [gl_cv___builtin_expect], [AC_LINK_IFELSE( [AC_LANG_SOURCE([[ int main (int argc, char **argv) { argc = __builtin_expect (argc, 100); return argv[argc != 100][0]; }]])], [gl_cv___builtin_expect=yes], [AC_LINK_IFELSE( [AC_LANG_SOURCE([[ #include int main (int argc, char **argv) { argc = __builtin_expect (argc, 100); return argv[argc != 100][0]; }]])], [gl_cv___builtin_expect="in "], [gl_cv___builtin_expect=no])])]) if test "$gl_cv___builtin_expect" = yes; then AC_DEFINE([HAVE___BUILTIN_EXPECT], [1]) elif test "$gl_cv___builtin_expect" = "in "; then AC_DEFINE([HAVE___BUILTIN_EXPECT], [2]) fi AH_VERBATIM([HAVE___BUILTIN_EXPECT], [/* Define to 1 if the compiler supports __builtin_expect, and to 2 if does. */ #undef HAVE___BUILTIN_EXPECT #ifndef HAVE___BUILTIN_EXPECT # define __builtin_expect(e, c) (e) #elif HAVE___BUILTIN_EXPECT == 2 # include #endif ]) ]) gnuastro-0.5/bootstrapped/m4/btowc.m40000644000175000017500000000647413217200022014547 00000000000000# btowc.m4 serial 11 dnl Copyright (C) 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_BTOWC], [ AC_REQUIRE([gl_WCHAR_H_DEFAULTS]) dnl Check whether is usable at all, first. Otherwise the test dnl program below may lead to an endless loop. See dnl . AC_REQUIRE([gl_WCHAR_H_INLINE_OK]) AC_CHECK_FUNCS_ONCE([btowc]) if test $ac_cv_func_btowc = no; then HAVE_BTOWC=0 else AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([gt_LOCALE_FR]) AC_REQUIRE([AC_CANONICAL_HOST]) dnl for cross-compiles dnl Cygwin 1.7.2 btowc('\0') is WEOF, not 0. AC_CACHE_CHECK([whether btowc(0) is correct], [gl_cv_func_btowc_nul], [ AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (btowc ('\0') != 0) return 1; return 0; }]])], [gl_cv_func_btowc_nul=yes], [gl_cv_func_btowc_nul=no], [ changequote(,)dnl case "$host_os" in # Guess no on Cygwin. cygwin*) gl_cv_func_btowc_nul="guessing no" ;; # Guess yes on native Windows. mingw*) gl_cv_func_btowc_nul="guessing yes" ;; # Guess yes otherwise. *) gl_cv_func_btowc_nul="guessing yes" ;; esac changequote([,])dnl ]) ]) dnl IRIX 6.5 btowc(EOF) is 0xFF, not WEOF. AC_CACHE_CHECK([whether btowc(EOF) is correct], [gl_cv_func_btowc_eof], [ dnl Initial guess, used when cross-compiling or when no suitable locale dnl is present. changequote(,)dnl case "$host_os" in # Guess no on IRIX. irix*) gl_cv_func_btowc_eof="guessing no" ;; # Guess yes on native Windows. mingw*) gl_cv_func_btowc_eof="guessing yes" ;; # Guess yes otherwise. *) gl_cv_func_btowc_eof="guessing yes" ;; esac changequote([,])dnl if test $LOCALE_FR != none; then AC_RUN_IFELSE( [AC_LANG_SOURCE([[ #include #include /* Tru64 with Desktop Toolkit C has a bug: must be included before . BSD/OS 4.0.1 has a bug: , and must be included before . */ #include #include #include #include int main () { if (setlocale (LC_ALL, "$LOCALE_FR") != NULL) { if (btowc (EOF) != WEOF) return 1; } return 0; }]])], [gl_cv_func_btowc_eof=yes], [gl_cv_func_btowc_eof=no], [:]) fi ]) case "$gl_cv_func_btowc_nul" in *yes) ;; *) REPLACE_BTOWC=1 ;; esac case "$gl_cv_func_btowc_eof" in *yes) ;; *) REPLACE_BTOWC=1 ;; esac fi ]) # Prerequisites of lib/btowc.c. AC_DEFUN([gl_PREREQ_BTOWC], [ : ]) gnuastro-0.5/bootstrapped/m4/ax_pthread.m40000644000175000017500000005052213217200050015542 00000000000000# =========================================================================== # https://www.gnu.org/software/autoconf-archive/ax_pthread.html # =========================================================================== # # SYNOPSIS # # AX_PTHREAD([ACTION-IF-FOUND[, ACTION-IF-NOT-FOUND]]) # # DESCRIPTION # # This macro figures out how to build C programs using POSIX threads. It # sets the PTHREAD_LIBS output variable to the threads library and linker # flags, and the PTHREAD_CFLAGS output variable to any special C compiler # flags that are needed. (The user can also force certain compiler # flags/libs to be tested by setting these environment variables.) # # Also sets PTHREAD_CC to any special C compiler that is needed for # multi-threaded programs (defaults to the value of CC otherwise). (This # is necessary on AIX to use the special cc_r compiler alias.) # # NOTE: You are assumed to not only compile your program with these flags, # but also to link with them as well. For example, you might link with # $PTHREAD_CC $CFLAGS $PTHREAD_CFLAGS $LDFLAGS ... $PTHREAD_LIBS $LIBS # # If you are only building threaded programs, you may wish to use these # variables in your default LIBS, CFLAGS, and CC: # # LIBS="$PTHREAD_LIBS $LIBS" # CFLAGS="$CFLAGS $PTHREAD_CFLAGS" # CC="$PTHREAD_CC" # # In addition, if the PTHREAD_CREATE_JOINABLE thread-attribute constant # has a nonstandard name, this macro defines PTHREAD_CREATE_JOINABLE to # that name (e.g. PTHREAD_CREATE_UNDETACHED on AIX). # # Also HAVE_PTHREAD_PRIO_INHERIT is defined if pthread is found and the # PTHREAD_PRIO_INHERIT symbol is defined when compiling with # PTHREAD_CFLAGS. # # ACTION-IF-FOUND is a list of shell commands to run if a threads library # is found, and ACTION-IF-NOT-FOUND is a list of commands to run it if it # is not found. If ACTION-IF-FOUND is not specified, the default action # will define HAVE_PTHREAD. # # Please let the authors know if this macro fails on any platform, or if # you have any other suggestions or comments. This macro was based on work # by SGJ on autoconf scripts for FFTW (http://www.fftw.org/) (with help # from M. Frigo), as well as ac_pthread and hb_pthread macros posted by # Alejandro Forero Cuervo to the autoconf macro repository. We are also # grateful for the helpful feedback of numerous users. # # Updated for Autoconf 2.68 by Daniel Richard G. # # LICENSE # # Copyright (c) 2008 Steven G. Johnson # Copyright (c) 2011 Daniel Richard G. # # This program is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # This program is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General # Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program. If not, see . # # As a special exception, the respective Autoconf Macro's copyright owner # gives unlimited permission to copy, distribute and modify the configure # scripts that are the output of Autoconf when processing the Macro. You # need not follow the terms of the GNU General Public License when using # or distributing such scripts, even though portions of the text of the # Macro appear in them. The GNU General Public License (GPL) does govern # all other use of the material that constitutes the Autoconf Macro. # # This special exception to the GPL applies to versions of the Autoconf # Macro released by the Autoconf Archive. When you make and distribute a # modified version of the Autoconf Macro, you may extend this special # exception to the GPL to apply to your modified version as well. #serial 24 AU_ALIAS([ACX_PTHREAD], [AX_PTHREAD]) AC_DEFUN([AX_PTHREAD], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_REQUIRE([AC_PROG_CC]) AC_REQUIRE([AC_PROG_SED]) AC_LANG_PUSH([C]) ax_pthread_ok=no # We used to check for pthread.h first, but this fails if pthread.h # requires special compiler flags (e.g. on Tru64 or Sequent). # It gets checked for in the link test anyway. # First of all, check if the user has set any of the PTHREAD_LIBS, # etcetera environment variables, and if threads linking works using # them: if test "x$PTHREAD_CFLAGS$PTHREAD_LIBS" != "x"; then ax_pthread_save_CC="$CC" ax_pthread_save_CFLAGS="$CFLAGS" ax_pthread_save_LIBS="$LIBS" AS_IF([test "x$PTHREAD_CC" != "x"], [CC="$PTHREAD_CC"]) CFLAGS="$CFLAGS $PTHREAD_CFLAGS" LIBS="$PTHREAD_LIBS $LIBS" AC_MSG_CHECKING([for pthread_join using $CC $PTHREAD_CFLAGS $PTHREAD_LIBS]) AC_LINK_IFELSE([AC_LANG_CALL([], [pthread_join])], [ax_pthread_ok=yes]) AC_MSG_RESULT([$ax_pthread_ok]) if test "x$ax_pthread_ok" = "xno"; then PTHREAD_LIBS="" PTHREAD_CFLAGS="" fi CC="$ax_pthread_save_CC" CFLAGS="$ax_pthread_save_CFLAGS" LIBS="$ax_pthread_save_LIBS" fi # We must check for the threads library under a number of different # names; the ordering is very important because some systems # (e.g. DEC) have both -lpthread and -lpthreads, where one of the # libraries is broken (non-POSIX). # Create a list of thread flags to try. Items starting with a "-" are # C compiler flags, and other items are library names, except for "none" # which indicates that we try without any flags at all, and "pthread-config" # which is a program returning the flags for the Pth emulation library. ax_pthread_flags="pthreads none -Kthread -pthread -pthreads -mthreads pthread --thread-safe -mt pthread-config" # The ordering *is* (sometimes) important. Some notes on the # individual items follow: # pthreads: AIX (must check this before -lpthread) # none: in case threads are in libc; should be tried before -Kthread and # other compiler flags to prevent continual compiler warnings # -Kthread: Sequent (threads in libc, but -Kthread needed for pthread.h) # -pthread: Linux/gcc (kernel threads), BSD/gcc (userland threads), Tru64 # (Note: HP C rejects this with "bad form for `-t' option") # -pthreads: Solaris/gcc (Note: HP C also rejects) # -mt: Sun Workshop C (may only link SunOS threads [-lthread], but it # doesn't hurt to check since this sometimes defines pthreads and # -D_REENTRANT too), HP C (must be checked before -lpthread, which # is present but should not be used directly; and before -mthreads, # because the compiler interprets this as "-mt" + "-hreads") # -mthreads: Mingw32/gcc, Lynx/gcc # pthread: Linux, etcetera # --thread-safe: KAI C++ # pthread-config: use pthread-config program (for GNU Pth library) case $host_os in freebsd*) # -kthread: FreeBSD kernel threads (preferred to -pthread since SMP-able) # lthread: LinuxThreads port on FreeBSD (also preferred to -pthread) ax_pthread_flags="-kthread lthread $ax_pthread_flags" ;; hpux*) # From the cc(1) man page: "[-mt] Sets various -D flags to enable # multi-threading and also sets -lpthread." ax_pthread_flags="-mt -pthread pthread $ax_pthread_flags" ;; openedition*) # IBM z/OS requires a feature-test macro to be defined in order to # enable POSIX threads at all, so give the user a hint if this is # not set. (We don't define these ourselves, as they can affect # other portions of the system API in unpredictable ways.) AC_EGREP_CPP([AX_PTHREAD_ZOS_MISSING], [ # if !defined(_OPEN_THREADS) && !defined(_UNIX03_THREADS) AX_PTHREAD_ZOS_MISSING # endif ], [AC_MSG_WARN([IBM z/OS requires -D_OPEN_THREADS or -D_UNIX03_THREADS to enable pthreads support.])]) ;; solaris*) # On Solaris (at least, for some versions), libc contains stubbed # (non-functional) versions of the pthreads routines, so link-based # tests will erroneously succeed. (N.B.: The stubs are missing # pthread_cleanup_push, or rather a function called by this macro, # so we could check for that, but who knows whether they'll stub # that too in a future libc.) So we'll check first for the # standard Solaris way of linking pthreads (-mt -lpthread). ax_pthread_flags="-mt,pthread pthread $ax_pthread_flags" ;; esac # GCC generally uses -pthread, or -pthreads on some platforms (e.g. SPARC) AS_IF([test "x$GCC" = "xyes"], [ax_pthread_flags="-pthread -pthreads $ax_pthread_flags"]) # The presence of a feature test macro requesting re-entrant function # definitions is, on some systems, a strong hint that pthreads support is # correctly enabled case $host_os in darwin* | hpux* | linux* | osf* | solaris*) ax_pthread_check_macro="_REENTRANT" ;; aix*) ax_pthread_check_macro="_THREAD_SAFE" ;; *) ax_pthread_check_macro="--" ;; esac AS_IF([test "x$ax_pthread_check_macro" = "x--"], [ax_pthread_check_cond=0], [ax_pthread_check_cond="!defined($ax_pthread_check_macro)"]) # Are we compiling with Clang? 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We could reasonably leave PTHREAD_CFLAGS empty. But # -pthread does define _REENTRANT, and while the Darwin headers # ignore this macro, third-party headers might not.) PTHREAD_CFLAGS="-pthread" PTHREAD_LIBS= ax_pthread_ok=yes # However, older versions of Clang make a point of warning the user # that, in an invocation where only linking and no compilation is # taking place, the -pthread option has no effect ("argument unused # during compilation"). They expect -pthread to be passed in only # when source code is being compiled. # # Problem is, this is at odds with the way Automake and most other # C build frameworks function, which is that the same flags used in # compilation (CFLAGS) are also used in linking. Many systems # supported by AX_PTHREAD require exactly this for POSIX threads # support, and in fact it is often not straightforward to specify a # flag that is used only in the compilation phase and not in # linking. Such a scenario is extremely rare in practice. # # Even though use of the -pthread flag in linking would only print # a warning, this can be a nuisance for well-run software projects # that build with -Werror. So if the active version of Clang has # this misfeature, we search for an option to squash it. AC_CACHE_CHECK([whether Clang needs flag to prevent "argument unused" warning when linking with -pthread], [ax_cv_PTHREAD_CLANG_NO_WARN_FLAG], [ax_cv_PTHREAD_CLANG_NO_WARN_FLAG=unknown # Create an alternate version of $ac_link that compiles and # links in two steps (.c -> .o, .o -> exe) instead of one # (.c -> exe), because the warning occurs only in the second # step ax_pthread_save_ac_link="$ac_link" ax_pthread_sed='s/conftest\.\$ac_ext/conftest.$ac_objext/g' ax_pthread_link_step=`$as_echo "$ac_link" | sed "$ax_pthread_sed"` ax_pthread_2step_ac_link="($ac_compile) && (echo ==== >&5) && ($ax_pthread_link_step)" ax_pthread_save_CFLAGS="$CFLAGS" for ax_pthread_try in '' -Qunused-arguments -Wno-unused-command-line-argument unknown; do AS_IF([test "x$ax_pthread_try" = "xunknown"], [break]) CFLAGS="-Werror -Wunknown-warning-option $ax_pthread_try -pthread $ax_pthread_save_CFLAGS" ac_link="$ax_pthread_save_ac_link" AC_LINK_IFELSE([AC_LANG_SOURCE([[int main(void){return 0;}]])], [ac_link="$ax_pthread_2step_ac_link" AC_LINK_IFELSE([AC_LANG_SOURCE([[int main(void){return 0;}]])], [break]) ]) done ac_link="$ax_pthread_save_ac_link" CFLAGS="$ax_pthread_save_CFLAGS" AS_IF([test "x$ax_pthread_try" = "x"], [ax_pthread_try=no]) ax_cv_PTHREAD_CLANG_NO_WARN_FLAG="$ax_pthread_try" ]) case "$ax_cv_PTHREAD_CLANG_NO_WARN_FLAG" in no | unknown) ;; *) PTHREAD_CFLAGS="$ax_cv_PTHREAD_CLANG_NO_WARN_FLAG $PTHREAD_CFLAGS" ;; esac fi # $ax_pthread_clang = yes if test "x$ax_pthread_ok" = "xno"; then for ax_pthread_try_flag in $ax_pthread_flags; do case $ax_pthread_try_flag in none) AC_MSG_CHECKING([whether pthreads work without any flags]) ;; -mt,pthread) AC_MSG_CHECKING([whether pthreads work with -mt -lpthread]) PTHREAD_CFLAGS="-mt" PTHREAD_LIBS="-lpthread" ;; -*) AC_MSG_CHECKING([whether pthreads work with $ax_pthread_try_flag]) PTHREAD_CFLAGS="$ax_pthread_try_flag" ;; pthread-config) AC_CHECK_PROG([ax_pthread_config], [pthread-config], [yes], [no]) AS_IF([test "x$ax_pthread_config" = "xno"], [continue]) PTHREAD_CFLAGS="`pthread-config --cflags`" PTHREAD_LIBS="`pthread-config --ldflags` `pthread-config --libs`" ;; *) AC_MSG_CHECKING([for the pthreads library -l$ax_pthread_try_flag]) PTHREAD_LIBS="-l$ax_pthread_try_flag" ;; esac ax_pthread_save_CFLAGS="$CFLAGS" ax_pthread_save_LIBS="$LIBS" CFLAGS="$CFLAGS $PTHREAD_CFLAGS" LIBS="$PTHREAD_LIBS $LIBS" # Check for various functions. We must include pthread.h, # since some functions may be macros. (On the Sequent, we # need a special flag -Kthread to make this header compile.) # We check for pthread_join because it is in -lpthread on IRIX # while pthread_create is in libc. We check for pthread_attr_init # due to DEC craziness with -lpthreads. We check for # pthread_cleanup_push because it is one of the few pthread # functions on Solaris that doesn't have a non-functional libc stub. # We try pthread_create on general principles. AC_LINK_IFELSE([AC_LANG_PROGRAM([#include # if $ax_pthread_check_cond # error "$ax_pthread_check_macro must be defined" # endif static void routine(void *a) { a = 0; } static void *start_routine(void *a) { return a; }], [pthread_t th; pthread_attr_t attr; pthread_create(&th, 0, start_routine, 0); pthread_join(th, 0); pthread_attr_init(&attr); pthread_cleanup_push(routine, 0); pthread_cleanup_pop(0) /* ; */])], [ax_pthread_ok=yes], []) CFLAGS="$ax_pthread_save_CFLAGS" LIBS="$ax_pthread_save_LIBS" AC_MSG_RESULT([$ax_pthread_ok]) AS_IF([test "x$ax_pthread_ok" = "xyes"], [break]) PTHREAD_LIBS="" PTHREAD_CFLAGS="" done fi # Various other checks: if test "x$ax_pthread_ok" = "xyes"; then ax_pthread_save_CFLAGS="$CFLAGS" ax_pthread_save_LIBS="$LIBS" CFLAGS="$CFLAGS $PTHREAD_CFLAGS" LIBS="$PTHREAD_LIBS $LIBS" # Detect AIX lossage: JOINABLE attribute is called UNDETACHED. AC_CACHE_CHECK([for joinable pthread attribute], [ax_cv_PTHREAD_JOINABLE_ATTR], [ax_cv_PTHREAD_JOINABLE_ATTR=unknown for ax_pthread_attr in PTHREAD_CREATE_JOINABLE PTHREAD_CREATE_UNDETACHED; do AC_LINK_IFELSE([AC_LANG_PROGRAM([#include ], [int attr = $ax_pthread_attr; return attr /* ; */])], [ax_cv_PTHREAD_JOINABLE_ATTR=$ax_pthread_attr; break], []) done ]) AS_IF([test "x$ax_cv_PTHREAD_JOINABLE_ATTR" != "xunknown" && \ test "x$ax_cv_PTHREAD_JOINABLE_ATTR" != "xPTHREAD_CREATE_JOINABLE" && \ test "x$ax_pthread_joinable_attr_defined" != "xyes"], [AC_DEFINE_UNQUOTED([PTHREAD_CREATE_JOINABLE], [$ax_cv_PTHREAD_JOINABLE_ATTR], [Define to necessary symbol if this constant uses a non-standard name on your system.]) ax_pthread_joinable_attr_defined=yes ]) AC_CACHE_CHECK([whether more special flags are required for pthreads], [ax_cv_PTHREAD_SPECIAL_FLAGS], [ax_cv_PTHREAD_SPECIAL_FLAGS=no case $host_os in solaris*) ax_cv_PTHREAD_SPECIAL_FLAGS="-D_POSIX_PTHREAD_SEMANTICS" ;; esac ]) AS_IF([test "x$ax_cv_PTHREAD_SPECIAL_FLAGS" != "xno" && \ test "x$ax_pthread_special_flags_added" != "xyes"], [PTHREAD_CFLAGS="$ax_cv_PTHREAD_SPECIAL_FLAGS $PTHREAD_CFLAGS" ax_pthread_special_flags_added=yes]) AC_CACHE_CHECK([for PTHREAD_PRIO_INHERIT], [ax_cv_PTHREAD_PRIO_INHERIT], [AC_LINK_IFELSE([AC_LANG_PROGRAM([[#include ]], [[int i = PTHREAD_PRIO_INHERIT;]])], [ax_cv_PTHREAD_PRIO_INHERIT=yes], [ax_cv_PTHREAD_PRIO_INHERIT=no]) ]) AS_IF([test "x$ax_cv_PTHREAD_PRIO_INHERIT" = "xyes" && \ test "x$ax_pthread_prio_inherit_defined" != "xyes"], [AC_DEFINE([HAVE_PTHREAD_PRIO_INHERIT], [1], [Have PTHREAD_PRIO_INHERIT.]) ax_pthread_prio_inherit_defined=yes ]) CFLAGS="$ax_pthread_save_CFLAGS" LIBS="$ax_pthread_save_LIBS" # More AIX lossage: compile with *_r variant if test "x$GCC" != "xyes"; then case $host_os in aix*) AS_CASE(["x/$CC"], [x*/c89|x*/c89_128|x*/c99|x*/c99_128|x*/cc|x*/cc128|x*/xlc|x*/xlc_v6|x*/xlc128|x*/xlc128_v6], [#handle absolute path differently from PATH based program lookup AS_CASE(["x$CC"], [x/*], [AS_IF([AS_EXECUTABLE_P([${CC}_r])],[PTHREAD_CC="${CC}_r"])], [AC_CHECK_PROGS([PTHREAD_CC],[${CC}_r],[$CC])])]) ;; esac fi fi test -n "$PTHREAD_CC" || PTHREAD_CC="$CC" AC_SUBST([PTHREAD_LIBS]) AC_SUBST([PTHREAD_CFLAGS]) AC_SUBST([PTHREAD_CC]) # Finally, execute ACTION-IF-FOUND/ACTION-IF-NOT-FOUND: if test "x$ax_pthread_ok" = "xyes"; then ifelse([$1],,[AC_DEFINE([HAVE_PTHREAD],[1],[Define if you have POSIX threads libraries and header files.])],[$1]) : else ax_pthread_ok=no $2 fi AC_LANG_POP ])dnl AX_PTHREAD gnuastro-0.5/bootstrapped/m4/ax_compare_version.m40000644000175000017500000001465313217200050017313 00000000000000# =========================================================================== # https://www.gnu.org/software/autoconf-archive/ax_compare_version.html # =========================================================================== # # SYNOPSIS # # AX_COMPARE_VERSION(VERSION_A, OP, VERSION_B, [ACTION-IF-TRUE], [ACTION-IF-FALSE]) # # DESCRIPTION # # This macro compares two version strings. Due to the various number of # minor-version numbers that can exist, and the fact that string # comparisons are not compatible with numeric comparisons, this is not # necessarily trivial to do in a autoconf script. This macro makes doing # these comparisons easy. # # The six basic comparisons are available, as well as checking equality # limited to a certain number of minor-version levels. # # The operator OP determines what type of comparison to do, and can be one # of: # # eq - equal (test A == B) # ne - not equal (test A != B) # le - less than or equal (test A <= B) # ge - greater than or equal (test A >= B) # lt - less than (test A < B) # gt - greater than (test A > B) # # Additionally, the eq and ne operator can have a number after it to limit # the test to that number of minor versions. # # eq0 - equal up to the length of the shorter version # ne0 - not equal up to the length of the shorter version # eqN - equal up to N sub-version levels # neN - not equal up to N sub-version levels # # When the condition is true, shell commands ACTION-IF-TRUE are run, # otherwise shell commands ACTION-IF-FALSE are run. The environment # variable 'ax_compare_version' is always set to either 'true' or 'false' # as well. # # Examples: # # AX_COMPARE_VERSION([3.15.7],[lt],[3.15.8]) # AX_COMPARE_VERSION([3.15],[lt],[3.15.8]) # # would both be true. # # AX_COMPARE_VERSION([3.15.7],[eq],[3.15.8]) # AX_COMPARE_VERSION([3.15],[gt],[3.15.8]) # # would both be false. # # AX_COMPARE_VERSION([3.15.7],[eq2],[3.15.8]) # # would be true because it is only comparing two minor versions. # # AX_COMPARE_VERSION([3.15.7],[eq0],[3.15]) # # would be true because it is only comparing the lesser number of minor # versions of the two values. # # Note: The characters that separate the version numbers do not matter. An # empty string is the same as version 0. OP is evaluated by autoconf, not # configure, so must be a string, not a variable. # # The author would like to acknowledge Guido Draheim whose advice about # the m4_case and m4_ifvaln functions make this macro only include the # portions necessary to perform the specific comparison specified by the # OP argument in the final configure script. # # LICENSE # # Copyright (c) 2008 Tim Toolan # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice # and this notice are preserved. This file is offered as-is, without any # warranty. #serial 13 dnl ######################################################################### AC_DEFUN([AX_COMPARE_VERSION], [ AC_REQUIRE([AC_PROG_AWK]) # Used to indicate true or false condition ax_compare_version=false # Convert the two version strings to be compared into a format that # allows a simple string comparison. The end result is that a version # string of the form 1.12.5-r617 will be converted to the form # 0001001200050617. In other words, each number is zero padded to four # digits, and non digits are removed. AS_VAR_PUSHDEF([A],[ax_compare_version_A]) A=`echo "$1" | sed -e 's/\([[0-9]]*\)/Z\1Z/g' \ -e 's/Z\([[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/[[^0-9]]//g'` AS_VAR_PUSHDEF([B],[ax_compare_version_B]) B=`echo "$3" | sed -e 's/\([[0-9]]*\)/Z\1Z/g' \ -e 's/Z\([[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/Z\([[0-9]][[0-9]][[0-9]]\)Z/Z0\1Z/g' \ -e 's/[[^0-9]]//g'` dnl # In the case of le, ge, lt, and gt, the strings are sorted as necessary dnl # then the first line is used to determine if the condition is true. dnl # The sed right after the echo is to remove any indented white space. m4_case(m4_tolower($2), [lt],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort -r | sed "s/x${A}/false/;s/x${B}/true/;1q"` ], [gt],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort | sed "s/x${A}/false/;s/x${B}/true/;1q"` ], [le],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort | sed "s/x${A}/true/;s/x${B}/false/;1q"` ], [ge],[ ax_compare_version=`echo "x$A x$B" | sed 's/^ *//' | sort -r | sed "s/x${A}/true/;s/x${B}/false/;1q"` ],[ dnl Split the operator from the subversion count if present. m4_bmatch(m4_substr($2,2), [0],[ # A count of zero means use the length of the shorter version. # Determine the number of characters in A and B. ax_compare_version_len_A=`echo "$A" | $AWK '{print(length)}'` ax_compare_version_len_B=`echo "$B" | $AWK '{print(length)}'` # Set A to no more than B's length and B to no more than A's length. A=`echo "$A" | sed "s/\(.\{$ax_compare_version_len_B\}\).*/\1/"` B=`echo "$B" | sed "s/\(.\{$ax_compare_version_len_A\}\).*/\1/"` ], [[0-9]+],[ # A count greater than zero means use only that many subversions A=`echo "$A" | sed "s/\(\([[0-9]]\{4\}\)\{m4_substr($2,2)\}\).*/\1/"` B=`echo "$B" | sed "s/\(\([[0-9]]\{4\}\)\{m4_substr($2,2)\}\).*/\1/"` ], [.+],[ AC_WARNING( [invalid OP numeric parameter: $2]) ],[]) # Pad zeros at end of numbers to make same length. ax_compare_version_tmp_A="$A`echo $B | sed 's/./0/g'`" B="$B`echo $A | sed 's/./0/g'`" A="$ax_compare_version_tmp_A" # Check for equality or inequality as necessary. m4_case(m4_tolower(m4_substr($2,0,2)), [eq],[ test "x$A" = "x$B" && ax_compare_version=true ], [ne],[ test "x$A" != "x$B" && ax_compare_version=true ],[ AC_WARNING([invalid OP parameter: $2]) ]) ]) AS_VAR_POPDEF([A])dnl AS_VAR_POPDEF([B])dnl dnl # Execute ACTION-IF-TRUE / ACTION-IF-FALSE. if test "$ax_compare_version" = "true" ; then m4_ifvaln([$4],[$4],[:])dnl m4_ifvaln([$5],[else $5])dnl fi ]) dnl AX_COMPARE_VERSION gnuastro-0.5/bootstrapped/m4/ax_check_compile_flag.m40000644000175000017500000000640313217200050017670 00000000000000# =========================================================================== # https://www.gnu.org/software/autoconf-archive/ax_check_compile_flag.html # =========================================================================== # # SYNOPSIS # # AX_CHECK_COMPILE_FLAG(FLAG, [ACTION-SUCCESS], [ACTION-FAILURE], [EXTRA-FLAGS], [INPUT]) # # DESCRIPTION # # Check whether the given FLAG works with the current language's compiler # or gives an error. (Warnings, however, are ignored) # # ACTION-SUCCESS/ACTION-FAILURE are shell commands to execute on # success/failure. # # If EXTRA-FLAGS is defined, it is added to the current language's default # flags (e.g. CFLAGS) when the check is done. The check is thus made with # the flags: "CFLAGS EXTRA-FLAGS FLAG". This can for example be used to # force the compiler to issue an error when a bad flag is given. # # INPUT gives an alternative input source to AC_COMPILE_IFELSE. # # NOTE: Implementation based on AX_CFLAGS_GCC_OPTION. Please keep this # macro in sync with AX_CHECK_{PREPROC,LINK}_FLAG. # # LICENSE # # Copyright (c) 2008 Guido U. Draheim # Copyright (c) 2011 Maarten Bosmans # # This program is free software: you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by the # Free Software Foundation, either version 3 of the License, or (at your # option) any later version. # # This program is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General # Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program. If not, see . # # As a special exception, the respective Autoconf Macro's copyright owner # gives unlimited permission to copy, distribute and modify the configure # scripts that are the output of Autoconf when processing the Macro. You # need not follow the terms of the GNU General Public License when using # or distributing such scripts, even though portions of the text of the # Macro appear in them. The GNU General Public License (GPL) does govern # all other use of the material that constitutes the Autoconf Macro. # # This special exception to the GPL applies to versions of the Autoconf # Macro released by the Autoconf Archive. When you make and distribute a # modified version of the Autoconf Macro, you may extend this special # exception to the GPL to apply to your modified version as well. #serial 5 AC_DEFUN([AX_CHECK_COMPILE_FLAG], [AC_PREREQ(2.64)dnl for _AC_LANG_PREFIX and AS_VAR_IF AS_VAR_PUSHDEF([CACHEVAR],[ax_cv_check_[]_AC_LANG_ABBREV[]flags_$4_$1])dnl AC_CACHE_CHECK([whether _AC_LANG compiler accepts $1], CACHEVAR, [ ax_check_save_flags=$[]_AC_LANG_PREFIX[]FLAGS _AC_LANG_PREFIX[]FLAGS="$[]_AC_LANG_PREFIX[]FLAGS $4 $1" AC_COMPILE_IFELSE([m4_default([$5],[AC_LANG_PROGRAM()])], [AS_VAR_SET(CACHEVAR,[yes])], [AS_VAR_SET(CACHEVAR,[no])]) _AC_LANG_PREFIX[]FLAGS=$ax_check_save_flags]) AS_VAR_IF(CACHEVAR,yes, [m4_default([$2], :)], [m4_default([$3], :)]) AS_VAR_POPDEF([CACHEVAR])dnl ])dnl AX_CHECK_COMPILE_FLAGS gnuastro-0.5/bootstrapped/m4/asm-underscore.m40000644000175000017500000000440213217200022016345 00000000000000# asm-underscore.m4 serial 3 dnl Copyright (C) 2010-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Bruno Haible. Based on as-underscore.m4 in GNU clisp. # gl_ASM_SYMBOL_PREFIX # Tests for the prefix of C symbols at the assembly language level and the # linker level. This prefix is either an underscore or empty. Defines the # C macro USER_LABEL_PREFIX to this prefix, and sets ASM_SYMBOL_PREFIX to # a stringified variant of this prefix. AC_DEFUN([gl_ASM_SYMBOL_PREFIX], [ dnl We don't use GCC's __USER_LABEL_PREFIX__ here, because dnl 1. It works only for GCC. dnl 2. It is incorrectly defined on some platforms, in some GCC versions. AC_REQUIRE([gl_C_ASM]) AC_CACHE_CHECK( [whether C symbols are prefixed with underscore at the linker level], [gl_cv_prog_as_underscore], [cat > conftest.c </dev/null 2>&1 if LC_ALL=C grep -E '(^|[[^a-zA-Z0-9_]])_foo([[^a-zA-Z0-9_]]|$)' conftest.$gl_asmext >/dev/null; then gl_cv_prog_as_underscore=yes else gl_cv_prog_as_underscore=no fi rm -f conftest* ]) if test $gl_cv_prog_as_underscore = yes; then USER_LABEL_PREFIX=_ else USER_LABEL_PREFIX= fi AC_DEFINE_UNQUOTED([USER_LABEL_PREFIX], [$USER_LABEL_PREFIX], [Define to the prefix of C symbols at the assembler and linker level, either an underscore or empty.]) ASM_SYMBOL_PREFIX='"'${USER_LABEL_PREFIX}'"' AC_SUBST([ASM_SYMBOL_PREFIX]) ]) # gl_C_ASM # Determines how to produce an assembly language file from C source code. # Sets the variables: # gl_asmext - the extension of assembly language output, # gl_c_asm_opt - the C compiler option that produces assembly language output. AC_DEFUN([gl_C_ASM], [ AC_EGREP_CPP([MicrosoftCompiler], [ #ifdef _MSC_VER MicrosoftCompiler #endif ], [gl_asmext='asm' gl_c_asm_opt='-c -Fa' ], [gl_asmext='s' gl_c_asm_opt='-S' ]) ]) gnuastro-0.5/bootstrapped/m4/arpa_inet_h.m40000644000175000017500000000357113217200022015675 00000000000000# arpa_inet_h.m4 serial 13 dnl Copyright (C) 2006, 2008-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl Written by Simon Josefsson and Bruno Haible AC_DEFUN([gl_HEADER_ARPA_INET], [ dnl Use AC_REQUIRE here, so that the default behavior below is expanded dnl once only, before all statements that occur in other macros. AC_REQUIRE([gl_ARPA_INET_H_DEFAULTS]) AC_CHECK_HEADERS_ONCE([arpa/inet.h]) if test $ac_cv_header_arpa_inet_h = yes; then HAVE_ARPA_INET_H=1 else HAVE_ARPA_INET_H=0 fi AC_SUBST([HAVE_ARPA_INET_H]) dnl is always overridden, because of GNULIB_POSIXCHECK. gl_CHECK_NEXT_HEADERS([arpa/inet.h]) AC_REQUIRE([gl_FEATURES_H]) dnl Check for declarations of anything we want to poison if the dnl corresponding gnulib module is not in use. gl_WARN_ON_USE_PREPARE([[ /* On some systems, this header is not self-consistent. */ #if !(defined __GLIBC__ || defined __UCLIBC__) # include #endif #ifdef __TANDEM # include #endif #include ]], [inet_ntop inet_pton]) ]) AC_DEFUN([gl_ARPA_INET_MODULE_INDICATOR], [ dnl Use AC_REQUIRE here, so that the default settings are expanded once only. AC_REQUIRE([gl_ARPA_INET_H_DEFAULTS]) gl_MODULE_INDICATOR_SET_VARIABLE([$1]) ]) AC_DEFUN([gl_ARPA_INET_H_DEFAULTS], [ GNULIB_INET_NTOP=0; AC_SUBST([GNULIB_INET_NTOP]) GNULIB_INET_PTON=0; AC_SUBST([GNULIB_INET_PTON]) dnl Assume proper GNU behavior unless another module says otherwise. HAVE_DECL_INET_NTOP=1; AC_SUBST([HAVE_DECL_INET_NTOP]) HAVE_DECL_INET_PTON=1; AC_SUBST([HAVE_DECL_INET_PTON]) REPLACE_INET_NTOP=0; AC_SUBST([REPLACE_INET_NTOP]) REPLACE_INET_PTON=0; AC_SUBST([REPLACE_INET_PTON]) ]) gnuastro-0.5/bootstrapped/m4/argp.m40000644000175000017500000000542613217200022014356 00000000000000# argp.m4 serial 15 dnl Copyright (C) 2003-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_ARGP], [ AC_REQUIRE([AC_C_INLINE]) AC_REQUIRE([AC_C_RESTRICT]) AC_REQUIRE([gl_USE_SYSTEM_EXTENSIONS]) AC_CHECK_DECLS([program_invocation_name], [], [AC_DEFINE([GNULIB_PROGRAM_INVOCATION_NAME], [1], [Define to 1 to add extern declaration of program_invocation_name to argp.h])], [[#include ]]) AC_CHECK_DECLS([program_invocation_short_name], [], [AC_DEFINE([GNULIB_PROGRAM_INVOCATION_SHORT_NAME], [1], [Define to 1 to add extern declaration of program_invocation_short_name to argp.h])], [[#include ]]) # Check if program_invocation_name and program_invocation_short_name # are defined elsewhere. It is improbable that only one of them will # be defined and other not, I prefer to stay on the safe side and to # test each one separately. AC_MSG_CHECKING([whether program_invocation_name is defined]) AC_LINK_IFELSE([AC_LANG_PROGRAM([[#include ]], [[program_invocation_name = "test";]])], [AC_DEFINE([HAVE_PROGRAM_INVOCATION_NAME], [1], [Define if program_invocation_name is defined]) AC_MSG_RESULT([yes])], [AC_MSG_RESULT([no])]) AC_MSG_CHECKING([whether program_invocation_short_name is defined]) AC_LINK_IFELSE([AC_LANG_PROGRAM([[#include ]], [[program_invocation_short_name = "test";]])], [AC_DEFINE([HAVE_PROGRAM_INVOCATION_SHORT_NAME], [1], [Define if program_invocation_short_name is defined]) AC_MSG_RESULT([yes])], [AC_MSG_RESULT([no])]) AC_CHECK_DECLS_ONCE([clearerr_unlocked]) AC_CHECK_DECLS_ONCE([feof_unlocked]) AC_CHECK_DECLS_ONCE([ferror_unlocked]) AC_CHECK_DECLS_ONCE([fflush_unlocked]) AC_CHECK_DECLS_ONCE([fgets_unlocked]) AC_CHECK_DECLS_ONCE([fputc_unlocked]) AC_CHECK_DECLS_ONCE([fputs_unlocked]) AC_CHECK_DECLS_ONCE([fread_unlocked]) AC_CHECK_DECLS_ONCE([fwrite_unlocked]) AC_CHECK_DECLS_ONCE([getc_unlocked]) AC_CHECK_DECLS_ONCE([getchar_unlocked]) AC_CHECK_DECLS_ONCE([putc_unlocked]) AC_CHECK_DECLS_ONCE([putchar_unlocked]) AC_CHECK_FUNCS_ONCE([flockfile funlockfile]) AC_CHECK_HEADERS_ONCE([features.h linewrap.h]) AC_REQUIRE([AC_FUNC_STRERROR_R]) ]) dnl argp-parse.c depends on GNU getopt internals, therefore use GNU getopt dnl always. AC_DEFUN([gl_REPLACE_GETOPT_ALWAYS], []) gnuastro-0.5/bootstrapped/m4/alloca.m40000644000175000017500000001037213217200022014654 00000000000000# alloca.m4 serial 14 dnl Copyright (C) 2002-2004, 2006-2007, 2009-2017 Free Software Foundation, dnl Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. AC_DEFUN([gl_FUNC_ALLOCA], [ AC_REQUIRE([AC_FUNC_ALLOCA]) if test $ac_cv_func_alloca_works = no; then gl_PREREQ_ALLOCA fi # Define an additional variable used in the Makefile substitution. if test $ac_cv_working_alloca_h = yes; then AC_CACHE_CHECK([for alloca as a compiler built-in], [gl_cv_rpl_alloca], [ AC_EGREP_CPP([Need own alloca], [ #if defined __GNUC__ || defined _AIX || defined _MSC_VER Need own alloca #endif ], [gl_cv_rpl_alloca=yes], [gl_cv_rpl_alloca=no]) ]) if test $gl_cv_rpl_alloca = yes; then dnl OK, alloca can be implemented through a compiler built-in. AC_DEFINE([HAVE_ALLOCA], [1], [Define to 1 if you have 'alloca' after including , a header that may be supplied by this distribution.]) ALLOCA_H=alloca.h else dnl alloca exists as a library function, i.e. it is slow and probably dnl a memory leak. Don't define HAVE_ALLOCA in this case. ALLOCA_H= fi else ALLOCA_H=alloca.h fi AC_SUBST([ALLOCA_H]) AM_CONDITIONAL([GL_GENERATE_ALLOCA_H], [test -n "$ALLOCA_H"]) ]) # Prerequisites of lib/alloca.c. # STACK_DIRECTION is already handled by AC_FUNC_ALLOCA. AC_DEFUN([gl_PREREQ_ALLOCA], [:]) # This works around a bug in autoconf <= 2.68. # See . m4_version_prereq([2.69], [] ,[ # This is taken from the following Autoconf patch: # https://git.savannah.gnu.org/gitweb/?p=autoconf.git;a=commitdiff;h=6cd9f12520b0d6f76d3230d7565feba1ecf29497 # _AC_LIBOBJ_ALLOCA # ----------------- # Set up the LIBOBJ replacement of 'alloca'. Well, not exactly # AC_LIBOBJ since we actually set the output variable 'ALLOCA'. # Nevertheless, for Automake, AC_LIBSOURCES it. m4_define([_AC_LIBOBJ_ALLOCA], [# The SVR3 libPW and SVR4 libucb both contain incompatible functions # that cause trouble. Some versions do not even contain alloca or # contain a buggy version. If you still want to use their alloca, # use ar to extract alloca.o from them instead of compiling alloca.c. AC_LIBSOURCES(alloca.c) AC_SUBST([ALLOCA], [\${LIBOBJDIR}alloca.$ac_objext])dnl AC_DEFINE(C_ALLOCA, 1, [Define to 1 if using 'alloca.c'.]) AC_CACHE_CHECK(whether 'alloca.c' needs Cray hooks, ac_cv_os_cray, [AC_EGREP_CPP(webecray, [#if defined CRAY && ! defined CRAY2 webecray #else wenotbecray #endif ], ac_cv_os_cray=yes, ac_cv_os_cray=no)]) if test $ac_cv_os_cray = yes; then for ac_func in _getb67 GETB67 getb67; do AC_CHECK_FUNC($ac_func, [AC_DEFINE_UNQUOTED(CRAY_STACKSEG_END, $ac_func, [Define to one of '_getb67', 'GETB67', 'getb67' for Cray-2 and Cray-YMP systems. This function is required for 'alloca.c' support on those systems.]) break]) done fi AC_CACHE_CHECK([stack direction for C alloca], [ac_cv_c_stack_direction], [AC_RUN_IFELSE([AC_LANG_SOURCE( [AC_INCLUDES_DEFAULT int find_stack_direction (int *addr, int depth) { int dir, dummy = 0; if (! addr) addr = &dummy; *addr = addr < &dummy ? 1 : addr == &dummy ? 0 : -1; dir = depth ? find_stack_direction (addr, depth - 1) : 0; return dir + dummy; } int main (int argc, char **argv) { return find_stack_direction (0, argc + !argv + 20) < 0; }])], [ac_cv_c_stack_direction=1], [ac_cv_c_stack_direction=-1], [ac_cv_c_stack_direction=0])]) AH_VERBATIM([STACK_DIRECTION], [/* If using the C implementation of alloca, define if you know the direction of stack growth for your system; otherwise it will be automatically deduced at runtime. STACK_DIRECTION > 0 => grows toward higher addresses STACK_DIRECTION < 0 => grows toward lower addresses STACK_DIRECTION = 0 => direction of growth unknown */ @%:@undef STACK_DIRECTION])dnl AC_DEFINE_UNQUOTED(STACK_DIRECTION, $ac_cv_c_stack_direction) ])# _AC_LIBOBJ_ALLOCA ]) gnuastro-0.5/bootstrapped/m4/absolute-header.m40000644000175000017500000001034713217200022016467 00000000000000# absolute-header.m4 serial 16 dnl Copyright (C) 2006-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl From Derek Price. # gl_ABSOLUTE_HEADER(HEADER1 HEADER2 ...) # --------------------------------------- # Find the absolute name of a header file, testing first if the header exists. # If the header were sys/inttypes.h, this macro would define # ABSOLUTE_SYS_INTTYPES_H to the '""' quoted absolute name of sys/inttypes.h # in config.h # (e.g. '#define ABSOLUTE_SYS_INTTYPES_H "///usr/include/sys/inttypes.h"'). # The three "///" are to pacify Sun C 5.8, which otherwise would say # "warning: #include of /usr/include/... may be non-portable". # Use '""', not '<>', so that the /// cannot be confused with a C99 comment. # Note: This macro assumes that the header file is not empty after # preprocessing, i.e. it does not only define preprocessor macros but also # provides some type/enum definitions or function/variable declarations. AC_DEFUN([gl_ABSOLUTE_HEADER], [AC_REQUIRE([AC_CANONICAL_HOST]) AC_LANG_PREPROC_REQUIRE()dnl dnl FIXME: gl_absolute_header and ac_header_exists must be used unquoted dnl until we can assume autoconf 2.64 or newer. m4_foreach_w([gl_HEADER_NAME], [$1], [AS_VAR_PUSHDEF([gl_absolute_header], [gl_cv_absolute_]m4_defn([gl_HEADER_NAME]))dnl AC_CACHE_CHECK([absolute name of <]m4_defn([gl_HEADER_NAME])[>], m4_defn([gl_absolute_header]), [AS_VAR_PUSHDEF([ac_header_exists], [ac_cv_header_]m4_defn([gl_HEADER_NAME]))dnl AC_CHECK_HEADERS_ONCE(m4_defn([gl_HEADER_NAME]))dnl if test AS_VAR_GET(ac_header_exists) = yes; then gl_ABSOLUTE_HEADER_ONE(m4_defn([gl_HEADER_NAME])) fi AS_VAR_POPDEF([ac_header_exists])dnl ])dnl AC_DEFINE_UNQUOTED(AS_TR_CPP([ABSOLUTE_]m4_defn([gl_HEADER_NAME])), ["AS_VAR_GET(gl_absolute_header)"], [Define this to an absolute name of <]m4_defn([gl_HEADER_NAME])[>.]) AS_VAR_POPDEF([gl_absolute_header])dnl ])dnl ])# gl_ABSOLUTE_HEADER # gl_ABSOLUTE_HEADER_ONE(HEADER) # ------------------------------ # Like gl_ABSOLUTE_HEADER, except that: # - it assumes that the header exists, # - it uses the current CPPFLAGS, # - it does not cache the result, # - it is silent. AC_DEFUN([gl_ABSOLUTE_HEADER_ONE], [ AC_REQUIRE([AC_CANONICAL_HOST]) AC_LANG_CONFTEST([AC_LANG_SOURCE([[#include <]]m4_dquote([$1])[[>]])]) dnl AIX "xlc -E" and "cc -E" omit #line directives for header files dnl that contain only a #include of other header files and no dnl non-comment tokens of their own. This leads to a failure to dnl detect the absolute name of , , dnl and others. The workaround is to force preservation of comments dnl through option -C. This ensures all necessary #line directives dnl are present. GCC supports option -C as well. case "$host_os" in aix*) gl_absname_cpp="$ac_cpp -C" ;; *) gl_absname_cpp="$ac_cpp" ;; esac changequote(,) case "$host_os" in mingw*) dnl For the sake of native Windows compilers (excluding gcc), dnl treat backslash as a directory separator, like /. dnl Actually, these compilers use a double-backslash as dnl directory separator, inside the dnl # line "filename" dnl directives. gl_dirsep_regex='[/\\]' ;; *) gl_dirsep_regex='\/' ;; esac dnl A sed expression that turns a string into a basic regular dnl expression, for use within "/.../". gl_make_literal_regex_sed='s,[]$^\\.*/[],\\&,g' gl_header_literal_regex=`echo '$1' \ | sed -e "$gl_make_literal_regex_sed"` gl_absolute_header_sed="/${gl_dirsep_regex}${gl_header_literal_regex}/"'{ s/.*"\(.*'"${gl_dirsep_regex}${gl_header_literal_regex}"'\)".*/\1/ s|^/[^/]|//&| p q }' changequote([,]) dnl eval is necessary to expand gl_absname_cpp. dnl Ultrix and Pyramid sh refuse to redirect output of eval, dnl so use subshell. AS_VAR_SET([gl_cv_absolute_]AS_TR_SH([[$1]]), [`(eval "$gl_absname_cpp conftest.$ac_ext") 2>&AS_MESSAGE_LOG_FD | sed -n "$gl_absolute_header_sed"`]) ]) gnuastro-0.5/bootstrapped/m4/00gnulib.m40000644000175000017500000000415213217200022015040 00000000000000# 00gnulib.m4 serial 3 dnl Copyright (C) 2009-2017 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl This file must be named something that sorts before all other dnl gnulib-provided .m4 files. It is needed until such time as we can dnl assume Autoconf 2.64, with its improved AC_DEFUN_ONCE and dnl m4_divert semantics. # Until autoconf 2.63, handling of the diversion stack required m4_init # to be called first; but this does not happen with aclocal. Wrapping # the entire execution in another layer of the diversion stack fixes this. # Worse, prior to autoconf 2.62, m4_wrap depended on the underlying m4 # for whether it was FIFO or LIFO; in order to properly balance with # m4_init, we need to undo our push just before anything wrapped within # the m4_init body. The way to ensure this is to wrap both sides of # m4_init with a one-shot macro that does the pop at the right time. m4_ifndef([_m4_divert_diversion], [m4_divert_push([KILL]) m4_define([gl_divert_fixup], [m4_divert_pop()m4_define([$0])]) m4_define([m4_init], [gl_divert_fixup()]m4_defn([m4_init])[gl_divert_fixup()])]) # AC_DEFUN_ONCE([NAME], VALUE) # ---------------------------- # Define NAME to expand to VALUE on the first use (whether by direct # expansion, or by AC_REQUIRE), and to nothing on all subsequent uses. # Avoid bugs in AC_REQUIRE in Autoconf 2.63 and earlier. This # definition is slower than the version in Autoconf 2.64, because it # can only use interfaces that existed since 2.59; but it achieves the # same effect. Quoting is necessary to avoid confusing Automake. m4_version_prereq([2.63.263], [], [m4_define([AC][_DEFUN_ONCE], [AC][_DEFUN([$1], [AC_REQUIRE([_gl_DEFUN_ONCE([$1])], [m4_indir([_gl_DEFUN_ONCE([$1])])])])]dnl [AC][_DEFUN([_gl_DEFUN_ONCE([$1])], [$2])])]) # gl_00GNULIB # ----------- # Witness macro that this file has been included. Needed to force # Automake to include this file prior to all other gnulib .m4 files. AC_DEFUN([gl_00GNULIB]) gnuastro-0.5/bootstrapped/build-aux/0000755000175000017500000000000013217220465014623 500000000000000gnuastro-0.5/bootstrapped/build-aux/test-driver0000755000175000017500000001104113217200071016725 00000000000000#! /bin/sh # test-driver - basic testsuite driver script. scriptversion=2016-01-11.22; # UTC # Copyright (C) 2011-2017 Free Software Foundation, Inc. # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to or send patches to # . # Make unconditional expansion of undefined variables an error. 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I.e., skip the test if it's "UNKNOWN" # or if it came from .tarball-version. if test "x$v_from_git" != x; then # Don't declare a version "dirty" merely because a timestamp has changed. git update-index --refresh > /dev/null 2>&1 dirty=`exec 2>/dev/null;git diff-index --name-only HEAD` || dirty= case "$dirty" in '') ;; *) # Append the suffix only if there isn't one already. case $v in *-dirty) ;; *) v="$v-dirty" ;; esac ;; esac fi # Omit the trailing newline, so that m4_esyscmd can use the result directly. printf %s "$v" # Local variables: # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-time-zone: "UTC0" # time-stamp-end: "; # UTC" # End: gnuastro-0.5/bootstrapped/build-aux/gendocs.sh0000755000175000017500000004110413217200020016505 00000000000000#!/bin/sh -e # gendocs.sh -- generate a GNU manual in many formats. This script is # mentioned in maintain.texi. See the help message below for usage details. scriptversion=2017-09-12.23 # Copyright 2003-2017 Free Software Foundation, Inc. # # This program is free software: you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 3 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see . # # Original author: Mohit Agarwal. # Send bug reports and any other correspondence to bug-gnulib@gnu.org. # # The latest version of this script, and the companion template, is # available from the Gnulib repository: # # https://git.savannah.gnu.org/cgit/gnulib.git/tree/build-aux/gendocs.sh # https://git.savannah.gnu.org/cgit/gnulib.git/tree/doc/gendocs_template # TODO: # - image importing was only implemented for HTML generated by # makeinfo. But it should be simple enough to adjust. # - images are not imported in the source tarball. All the needed # formats (PDF, PNG, etc.) should be included. prog=`basename "$0"` srcdir=`pwd` scripturl="https://git.savannah.gnu.org/cgit/gnulib.git/plain/build-aux/gendocs.sh" templateurl="https://git.savannah.gnu.org/cgit/gnulib.git/plain/doc/gendocs_template" : ${SETLANG="env LANG= LC_MESSAGES= LC_ALL= LANGUAGE="} : ${MAKEINFO="makeinfo"} : ${TEXI2DVI="texi2dvi"} : ${DOCBOOK2HTML="docbook2html"} : ${DOCBOOK2PDF="docbook2pdf"} : ${DOCBOOK2TXT="docbook2txt"} : ${GENDOCS_TEMPLATE_DIR="."} : ${PERL='perl'} : ${TEXI2HTML="texi2html"} unset CDPATH unset use_texi2html MANUAL_TITLE= PACKAGE= EMAIL=webmasters@gnu.org # please override with --email commonarg= # passed to all makeinfo/texi2html invcations. dirargs= # passed to all tools (-I dir). dirs= # -I directories. htmlarg="--css-ref=/software/gnulib/manual.css -c TOP_NODE_UP_URL=/manual" infoarg=--no-split generate_ascii=true generate_html=true generate_info=true generate_tex=true outdir=manual source_extra= split=node srcfile= texarg="-t @finalout" version="gendocs.sh $scriptversion Copyright 2017 Free Software Foundation, Inc. There is NO warranty. You may redistribute this software under the terms of the GNU General Public License. For more information about these matters, see the files named COPYING." usage="Usage: $prog [OPTION]... PACKAGE MANUAL-TITLE Generate output in various formats from PACKAGE.texinfo (or .texi or .txi) source. See the GNU Maintainers document for a more extensive discussion: https://www.gnu.org/prep/maintain_toc.html Options: --email ADR use ADR as contact in generated web pages; always give this. -s SRCFILE read Texinfo from SRCFILE, instead of PACKAGE.{texinfo|texi|txi} -o OUTDIR write files into OUTDIR, instead of manual/. -I DIR append DIR to the Texinfo search path. --common ARG pass ARG in all invocations. --html ARG pass ARG to makeinfo or texi2html for HTML targets, instead of '$htmlarg'. --info ARG pass ARG to makeinfo for Info, instead of --no-split. --no-ascii skip generating the plain text output. --no-html skip generating the html output. --no-info skip generating the info output. --no-tex skip generating the dvi and pdf output. --source ARG include ARG in tar archive of sources. --split HOW make split HTML by node, section, chapter; default node. --tex ARG pass ARG to texi2dvi for DVI and PDF, instead of -t @finalout. --texi2html use texi2html to make HTML target, with all split versions. --docbook convert through DocBook too (xml, txt, html, pdf). --help display this help and exit successfully. --version display version information and exit successfully. Simple example: $prog --email bug-gnu-emacs@gnu.org emacs \"GNU Emacs Manual\" Typical sequence: cd PACKAGESOURCE/doc wget \"$scripturl\" wget \"$templateurl\" $prog --email BUGLIST MANUAL \"GNU MANUAL - One-line description\" Output will be in a new subdirectory \"manual\" (by default; use -o OUTDIR to override). Move all the new files into your web CVS tree, as explained in the Web Pages node of maintain.texi. Please use the --email ADDRESS option so your own bug-reporting address will be used in the generated HTML pages. MANUAL-TITLE is included as part of the HTML of the overall manual/index.html file. It should include the name of the package being documented. manual/index.html is created by substitution from the file $GENDOCS_TEMPLATE_DIR/gendocs_template. (Feel free to modify the generic template for your own purposes.) If you have several manuals, you'll need to run this script several times with different MANUAL values, specifying a different output directory with -o each time. Then write (by hand) an overall index.html with links to them all. If a manual's Texinfo sources are spread across several directories, first copy or symlink all Texinfo sources into a single directory. (Part of the script's work is to make a tar.gz of the sources.) As implied above, by default monolithic Info files are generated. If you want split Info, or other Info options, use --info to override. You can set the environment variables MAKEINFO, TEXI2DVI, TEXI2HTML, and PERL to control the programs that get executed, and GENDOCS_TEMPLATE_DIR to control where the gendocs_template file is looked for. With --docbook, the environment variables DOCBOOK2HTML, DOCBOOK2PDF, and DOCBOOK2TXT are also consulted. By default, makeinfo and texi2dvi are run in the default (English) locale, since that's the language of most Texinfo manuals. If you happen to have a non-English manual and non-English web site, see the SETLANG setting in the source. Email bug reports or enhancement requests to bug-gnulib@gnu.org. " while test $# -gt 0; do case $1 in -s) shift; srcfile=$1;; -o) shift; outdir=$1;; -I) shift; dirargs="$dirargs -I '$1'"; dirs="$dirs $1";; --common) shift; commonarg=$1;; --docbook) docbook=yes;; --email) shift; EMAIL=$1;; --html) shift; htmlarg=$1;; --info) shift; infoarg=$1;; --no-ascii) generate_ascii=false;; --no-html) generate_ascii=false;; --no-info) generate_info=false;; --no-tex) generate_tex=false;; --source) shift; source_extra=$1;; --split) shift; split=$1;; --tex) shift; texarg=$1;; --texi2html) use_texi2html=1;; --help) echo "$usage"; exit 0;; --version) echo "$version"; exit 0;; -*) echo "$0: Unknown option \`$1'." >&2 echo "$0: Try \`--help' for more information." >&2 exit 1;; *) if test -z "$PACKAGE"; then PACKAGE=$1 elif test -z "$MANUAL_TITLE"; then MANUAL_TITLE=$1 else echo "$0: extra non-option argument \`$1'." >&2 exit 1 fi;; esac shift done # makeinfo uses the dirargs, but texi2dvi doesn't. commonarg=" $dirargs $commonarg" # For most of the following, the base name is just $PACKAGE base=$PACKAGE if test -n "$srcfile"; then # but here, we use the basename of $srcfile base=`basename "$srcfile"` case $base in *.txi|*.texi|*.texinfo) base=`echo "$base"|sed 's/\.[texinfo]*$//'`;; esac PACKAGE=$base elif test -s "$srcdir/$PACKAGE.texinfo"; then srcfile=$srcdir/$PACKAGE.texinfo elif test -s "$srcdir/$PACKAGE.texi"; then srcfile=$srcdir/$PACKAGE.texi elif test -s "$srcdir/$PACKAGE.txi"; then srcfile=$srcdir/$PACKAGE.txi else echo "$0: cannot find .texinfo or .texi or .txi for $PACKAGE in $srcdir." >&2 exit 1 fi if test ! -r $GENDOCS_TEMPLATE_DIR/gendocs_template; then echo "$0: cannot read $GENDOCS_TEMPLATE_DIR/gendocs_template." >&2 echo "$0: it is available from $templateurl." >&2 exit 1 fi # Function to return size of $1 in something resembling kilobytes. calcsize() { size=`ls -ksl $1 | awk '{print $1}'` echo $size } # copy_images OUTDIR HTML-FILE... # ------------------------------- # Copy all the images needed by the HTML-FILEs into OUTDIR. # Look for them in . and the -I directories; this is simpler than what # makeinfo supports with -I, but hopefully it will suffice. copy_images() { local odir odir=$1 shift $PERL -n -e " BEGIN { \$me = '$prog'; \$odir = '$odir'; @dirs = qw(. $dirs); } " -e ' /<img src="(.*?)"/g && ++$need{$1}; END { #print "$me: @{[keys %need]}\n"; # for debugging, show images found. FILE: for my $f (keys %need) { for my $d (@dirs) { if (-f "$d/$f") { use File::Basename; my $dest = dirname ("$odir/$f"); # use File::Path; -d $dest || mkpath ($dest) || die "$me: cannot mkdir $dest: $!\n"; # use File::Copy; copy ("$d/$f", $dest) || die "$me: cannot copy $d/$f to $dest: $!\n"; next FILE; } } die "$me: $ARGV: cannot find image $f\n"; } } ' -- "$@" || exit 1 } case $outdir in /*) abs_outdir=$outdir;; *) abs_outdir=$srcdir/$outdir;; esac echo "Making output for $srcfile" echo " in `pwd`" mkdir -p "$outdir/" # if $generate_info; then cmd="$SETLANG $MAKEINFO -o $PACKAGE.info $commonarg $infoarg \"$srcfile\"" echo "Generating info... ($cmd)" rm -f $PACKAGE.info* # get rid of any strays eval "$cmd" tar czf "$outdir/$PACKAGE.info.tar.gz" $PACKAGE.info* ls -l "$outdir/$PACKAGE.info.tar.gz" info_tgz_size=`calcsize "$outdir/$PACKAGE.info.tar.gz"` # do not mv the info files, there's no point in having them available # separately on the web. fi # end info # if $generate_tex; then cmd="$SETLANG $TEXI2DVI $dirargs $texarg \"$srcfile\"" printf "\nGenerating dvi... ($cmd)\n" eval "$cmd" # compress/finish dvi: gzip -f -9 $PACKAGE.dvi dvi_gz_size=`calcsize $PACKAGE.dvi.gz` mv $PACKAGE.dvi.gz "$outdir/" ls -l "$outdir/$PACKAGE.dvi.gz" cmd="$SETLANG $TEXI2DVI --pdf $dirargs $texarg \"$srcfile\"" printf "\nGenerating pdf... ($cmd)\n" eval "$cmd" pdf_size=`calcsize $PACKAGE.pdf` mv $PACKAGE.pdf "$outdir/" ls -l "$outdir/$PACKAGE.pdf" fi # end tex (dvi + pdf) # if $generate_ascii; then opt="-o $PACKAGE.txt --no-split --no-headers $commonarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\"" printf "\nGenerating ascii... ($cmd)\n" eval "$cmd" ascii_size=`calcsize $PACKAGE.txt` gzip -f -9 -c $PACKAGE.txt >"$outdir/$PACKAGE.txt.gz" ascii_gz_size=`calcsize "$outdir/$PACKAGE.txt.gz"` mv $PACKAGE.txt "$outdir/" ls -l "$outdir/$PACKAGE.txt" "$outdir/$PACKAGE.txt.gz" fi # if $generate_html; then # Split HTML at level $1. Used for texi2html. html_split() { opt="--split=$1 --node-files $commonarg $htmlarg" cmd="$SETLANG $TEXI2HTML --output $PACKAGE.html $opt \"$srcfile\"" printf "\nGenerating html by $1... ($cmd)\n" eval "$cmd" split_html_dir=$PACKAGE.html ( cd ${split_html_dir} || exit 1 ln -sf ${PACKAGE}.html index.html tar -czf "$abs_outdir/${PACKAGE}.html_$1.tar.gz" -- *.html ) eval html_$1_tgz_size=`calcsize "$outdir/${PACKAGE}.html_$1.tar.gz"` rm -f "$outdir"/html_$1/*.html mkdir -p "$outdir/html_$1/" mv ${split_html_dir}/*.html "$outdir/html_$1/" rmdir ${split_html_dir} } if test -z "$use_texi2html"; then opt="--no-split --html -o $PACKAGE.html $commonarg $htmlarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\"" printf "\nGenerating monolithic html... ($cmd)\n" rm -rf $PACKAGE.html # in case a directory is left over eval "$cmd" html_mono_size=`calcsize $PACKAGE.html` gzip -f -9 -c $PACKAGE.html >"$outdir/$PACKAGE.html.gz" html_mono_gz_size=`calcsize "$outdir/$PACKAGE.html.gz"` copy_images "$outdir/" $PACKAGE.html mv $PACKAGE.html "$outdir/" ls -l "$outdir/$PACKAGE.html" "$outdir/$PACKAGE.html.gz" # Before Texinfo 5.0, makeinfo did not accept a --split=HOW option, # it just always split by node. So if we're splitting by node anyway, # leave it out. if test "x$split" = xnode; then split_arg= else split_arg=--split=$split fi # opt="--html -o $PACKAGE.html $split_arg $commonarg $htmlarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\"" printf "\nGenerating html by $split... ($cmd)\n" eval "$cmd" split_html_dir=$PACKAGE.html copy_images $split_html_dir/ $split_html_dir/*.html ( cd $split_html_dir || exit 1 tar -czf "$abs_outdir/$PACKAGE.html_$split.tar.gz" -- * ) eval \ html_${split}_tgz_size=`calcsize "$outdir/$PACKAGE.html_$split.tar.gz"` rm -rf "$outdir/html_$split/" mv $split_html_dir "$outdir/html_$split/" du -s "$outdir/html_$split/" ls -l "$outdir/$PACKAGE.html_$split.tar.gz" else # use texi2html: opt="--output $PACKAGE.html $commonarg $htmlarg" cmd="$SETLANG $TEXI2HTML $opt \"$srcfile\"" printf "\nGenerating monolithic html with texi2html... ($cmd)\n" rm -rf $PACKAGE.html # in case a directory is left over eval "$cmd" html_mono_size=`calcsize $PACKAGE.html` gzip -f -9 -c $PACKAGE.html >"$outdir/$PACKAGE.html.gz" html_mono_gz_size=`calcsize "$outdir/$PACKAGE.html.gz"` mv $PACKAGE.html "$outdir/" html_split node html_split chapter html_split section fi fi # end html # printf "\nMaking .tar.gz for sources...\n" d=`dirname $srcfile` ( cd "$d" srcfiles=`ls -d *.texinfo *.texi *.txi *.eps $source_extra 2>/dev/null` || true tar czfh "$abs_outdir/$PACKAGE.texi.tar.gz" $srcfiles ls -l "$abs_outdir/$PACKAGE.texi.tar.gz" ) texi_tgz_size=`calcsize "$outdir/$PACKAGE.texi.tar.gz"` # # Do everything again through docbook. if test -n "$docbook"; then opt="-o - --docbook $commonarg" cmd="$SETLANG $MAKEINFO $opt \"$srcfile\" >${srcdir}/$PACKAGE-db.xml" printf "\nGenerating docbook XML... ($cmd)\n" eval "$cmd" docbook_xml_size=`calcsize $PACKAGE-db.xml` gzip -f -9 -c $PACKAGE-db.xml >"$outdir/$PACKAGE-db.xml.gz" docbook_xml_gz_size=`calcsize "$outdir/$PACKAGE-db.xml.gz"` mv $PACKAGE-db.xml "$outdir/" split_html_db_dir=html_node_db opt="$commonarg -o $split_html_db_dir" cmd="$DOCBOOK2HTML $opt \"${outdir}/$PACKAGE-db.xml\"" printf "\nGenerating docbook HTML... ($cmd)\n" eval "$cmd" ( cd ${split_html_db_dir} || exit 1 tar -czf "$abs_outdir/${PACKAGE}.html_node_db.tar.gz" -- *.html ) html_node_db_tgz_size=`calcsize "$outdir/${PACKAGE}.html_node_db.tar.gz"` rm -f "$outdir"/html_node_db/*.html mkdir -p "$outdir/html_node_db" mv ${split_html_db_dir}/*.html "$outdir/html_node_db/" rmdir ${split_html_db_dir} cmd="$DOCBOOK2TXT \"${outdir}/$PACKAGE-db.xml\"" printf "\nGenerating docbook ASCII... ($cmd)\n" eval "$cmd" docbook_ascii_size=`calcsize $PACKAGE-db.txt` mv $PACKAGE-db.txt "$outdir/" cmd="$DOCBOOK2PDF \"${outdir}/$PACKAGE-db.xml\"" printf "\nGenerating docbook PDF... ($cmd)\n" eval "$cmd" docbook_pdf_size=`calcsize $PACKAGE-db.pdf` mv $PACKAGE-db.pdf "$outdir/" fi # printf "\nMaking index.html for $PACKAGE...\n" if test -z "$use_texi2html"; then CONDS="/%%IF *HTML_SECTION%%/,/%%ENDIF *HTML_SECTION%%/d;\ /%%IF *HTML_CHAPTER%%/,/%%ENDIF *HTML_CHAPTER%%/d" else # should take account of --split here. CONDS="/%%ENDIF.*%%/d;/%%IF *HTML_SECTION%%/d;/%%IF *HTML_CHAPTER%%/d" fi curdate=`$SETLANG date '+%B %d, %Y'` sed \ -e "s!%%TITLE%%!$MANUAL_TITLE!g" \ -e "s!%%EMAIL%%!$EMAIL!g" \ -e "s!%%PACKAGE%%!$PACKAGE!g" \ -e "s!%%DATE%%!$curdate!g" \ -e "s!%%HTML_MONO_SIZE%%!$html_mono_size!g" \ -e "s!%%HTML_MONO_GZ_SIZE%%!$html_mono_gz_size!g" \ -e "s!%%HTML_NODE_TGZ_SIZE%%!$html_node_tgz_size!g" \ -e "s!%%HTML_SECTION_TGZ_SIZE%%!$html_section_tgz_size!g" \ -e "s!%%HTML_CHAPTER_TGZ_SIZE%%!$html_chapter_tgz_size!g" \ -e "s!%%INFO_TGZ_SIZE%%!$info_tgz_size!g" \ -e "s!%%DVI_GZ_SIZE%%!$dvi_gz_size!g" \ -e "s!%%PDF_SIZE%%!$pdf_size!g" \ -e "s!%%ASCII_SIZE%%!$ascii_size!g" \ -e "s!%%ASCII_GZ_SIZE%%!$ascii_gz_size!g" \ -e "s!%%TEXI_TGZ_SIZE%%!$texi_tgz_size!g" \ -e "s!%%DOCBOOK_HTML_NODE_TGZ_SIZE%%!$html_node_db_tgz_size!g" \ -e "s!%%DOCBOOK_ASCII_SIZE%%!$docbook_ascii_size!g" \ -e "s!%%DOCBOOK_PDF_SIZE%%!$docbook_pdf_size!g" \ -e "s!%%DOCBOOK_XML_SIZE%%!$docbook_xml_size!g" \ -e "s!%%DOCBOOK_XML_GZ_SIZE%%!$docbook_xml_gz_size!g" \ -e "s,%%SCRIPTURL%%,$scripturl,g" \ -e "s!%%SCRIPTNAME%%!$prog!g" \ -e "$CONDS" \ $GENDOCS_TEMPLATE_DIR/gendocs_template >"$outdir/index.html" echo "Done, see $outdir/ subdirectory for new files." # Local variables: # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-end: "$" # End: ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bootstrapped/build-aux/texinfo.tex�����������������������������������������������������0000644�0001750�0001750�00001350454�13216277135�016762� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������% texinfo.tex -- TeX macros to handle Texinfo files. % % Load plain if necessary, i.e., if running under initex. \expandafter\ifx\csname fmtname\endcsname\relax\input plain\fi % \def\texinfoversion{2017-12-18.20} % % Copyright 1985, 1986, 1988, 1990, 1991, 1992, 1993, 1994, 1995, % 1996, 1997, 1998, 1999, 2000, 2001, 2002, 2003, 2004, 2005, 2006, % 2007, 2008, 2009, 2010, 2011, 2012, 2013, 2014, 2015, 2016, 2017 % Free Software Foundation, Inc. % % This texinfo.tex file is free software: you can redistribute it and/or % modify it under the terms of the GNU General Public License as % published by the Free Software Foundation, either version 3 of the % License, or (at your option) any later version. % % This texinfo.tex file is distributed in the hope that it will be % useful, but WITHOUT ANY WARRANTY; without even the implied warranty % of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU % General Public License for more details. % % You should have received a copy of the GNU General Public License % along with this program. If not, see <https://www.gnu.org/licenses/>. % % As a special exception, when this file is read by TeX when processing % a Texinfo source document, you may use the result without % restriction. This Exception is an additional permission under section 7 % of the GNU General Public License, version 3 ("GPLv3"). % % Please try the latest version of texinfo.tex before submitting bug % reports; you can get the latest version from: % https://ftp.gnu.org/gnu/texinfo/ (the Texinfo release area), or % https://ftpmirror.gnu.org/texinfo/ (same, via a mirror), or % https://www.gnu.org/software/texinfo/ (the Texinfo home page) % The texinfo.tex in any given distribution could well be out % of date, so if that's what you're using, please check. % % Send bug reports to bug-texinfo@gnu.org. Please include including a % complete document in each bug report with which we can reproduce the % problem. Patches are, of course, greatly appreciated. % % To process a Texinfo manual with TeX, it's most reliable to use the % texi2dvi shell script that comes with the distribution. For a simple % manual foo.texi, however, you can get away with this: % tex foo.texi % texindex foo.?? % tex foo.texi % tex foo.texi % dvips foo.dvi -o # or whatever; this makes foo.ps. % The extra TeX runs get the cross-reference information correct. % Sometimes one run after texindex suffices, and sometimes you need more % than two; texi2dvi does it as many times as necessary. % % It is possible to adapt texinfo.tex for other languages, to some % extent. You can get the existing language-specific files from the % full Texinfo distribution. % % The GNU Texinfo home page is https://www.gnu.org/software/texinfo. \message{Loading texinfo [version \texinfoversion]:} % If in a .fmt file, print the version number % and turn on active characters that we couldn't do earlier because % they might have appeared in the input file name. \everyjob{\message{[Texinfo version \texinfoversion]}% \catcode`+=\active \catcode`\_=\active} % LaTeX's \typeout. This ensures that the messages it is used for % are identical in format to the corresponding ones from latex/pdflatex. \def\typeout{\immediate\write17}% \chardef\other=12 % We never want plain's \outer definition of \+ in Texinfo. % For @tex, we can use \tabalign. \let\+ = \relax % Save some plain tex macros whose names we will redefine. \let\ptexb=\b \let\ptexbullet=\bullet \let\ptexc=\c \let\ptexcomma=\, \let\ptexdot=\. \let\ptexdots=\dots \let\ptexend=\end \let\ptexequiv=\equiv \let\ptexexclam=\! \let\ptexfootnote=\footnote \let\ptexgtr=> \let\ptexhat=^ \let\ptexi=\i \let\ptexindent=\indent \let\ptexinsert=\insert \let\ptexlbrace=\{ \let\ptexless=< \let\ptexnewwrite\newwrite \let\ptexnoindent=\noindent \let\ptexplus=+ \let\ptexraggedright=\raggedright \let\ptexrbrace=\} \let\ptexslash=\/ \let\ptexsp=\sp \let\ptexstar=\* \let\ptexsup=\sup \let\ptext=\t \let\ptextop=\top {\catcode`\'=\active \global\let\ptexquoteright'}% active in plain's math mode % If this character appears in an error message or help string, it % starts a new line in the output. \newlinechar = `^^J % Use TeX 3.0's \inputlineno to get the line number, for better error % messages, but if we're using an old version of TeX, don't do anything. % \ifx\inputlineno\thisisundefined \let\linenumber = \empty % Pre-3.0. \else \def\linenumber{l.\the\inputlineno:\space} \fi % Set up fixed words for English if not already set. \ifx\putwordAppendix\undefined \gdef\putwordAppendix{Appendix}\fi \ifx\putwordChapter\undefined \gdef\putwordChapter{Chapter}\fi \ifx\putworderror\undefined \gdef\putworderror{error}\fi \ifx\putwordfile\undefined \gdef\putwordfile{file}\fi \ifx\putwordin\undefined \gdef\putwordin{in}\fi \ifx\putwordIndexIsEmpty\undefined \gdef\putwordIndexIsEmpty{(Index is empty)}\fi \ifx\putwordIndexNonexistent\undefined \gdef\putwordIndexNonexistent{(Index is nonexistent)}\fi \ifx\putwordInfo\undefined \gdef\putwordInfo{Info}\fi \ifx\putwordInstanceVariableof\undefined \gdef\putwordInstanceVariableof{Instance Variable of}\fi \ifx\putwordMethodon\undefined \gdef\putwordMethodon{Method on}\fi \ifx\putwordNoTitle\undefined \gdef\putwordNoTitle{No Title}\fi \ifx\putwordof\undefined \gdef\putwordof{of}\fi \ifx\putwordon\undefined \gdef\putwordon{on}\fi \ifx\putwordpage\undefined \gdef\putwordpage{page}\fi \ifx\putwordsection\undefined \gdef\putwordsection{section}\fi \ifx\putwordSection\undefined \gdef\putwordSection{Section}\fi \ifx\putwordsee\undefined \gdef\putwordsee{see}\fi \ifx\putwordSee\undefined \gdef\putwordSee{See}\fi \ifx\putwordShortTOC\undefined \gdef\putwordShortTOC{Short Contents}\fi \ifx\putwordTOC\undefined \gdef\putwordTOC{Table of Contents}\fi % \ifx\putwordMJan\undefined \gdef\putwordMJan{January}\fi \ifx\putwordMFeb\undefined \gdef\putwordMFeb{February}\fi \ifx\putwordMMar\undefined \gdef\putwordMMar{March}\fi \ifx\putwordMApr\undefined \gdef\putwordMApr{April}\fi \ifx\putwordMMay\undefined \gdef\putwordMMay{May}\fi \ifx\putwordMJun\undefined \gdef\putwordMJun{June}\fi \ifx\putwordMJul\undefined \gdef\putwordMJul{July}\fi \ifx\putwordMAug\undefined \gdef\putwordMAug{August}\fi \ifx\putwordMSep\undefined \gdef\putwordMSep{September}\fi \ifx\putwordMOct\undefined \gdef\putwordMOct{October}\fi \ifx\putwordMNov\undefined \gdef\putwordMNov{November}\fi \ifx\putwordMDec\undefined \gdef\putwordMDec{December}\fi % \ifx\putwordDefmac\undefined \gdef\putwordDefmac{Macro}\fi \ifx\putwordDefspec\undefined \gdef\putwordDefspec{Special Form}\fi \ifx\putwordDefvar\undefined \gdef\putwordDefvar{Variable}\fi \ifx\putwordDefopt\undefined \gdef\putwordDefopt{User Option}\fi \ifx\putwordDeffunc\undefined \gdef\putwordDeffunc{Function}\fi % Give the space character the catcode for a space. \def\spaceisspace{\catcode`\ =10\relax} % Likewise for ^^M, the end of line character. \def\endlineisspace{\catcode13=10\relax} \chardef\dashChar = `\- \chardef\slashChar = `\/ \chardef\underChar = `\_ % Ignore a token. % \def\gobble#1{} % The following is used inside several \edef's. \def\makecsname#1{\expandafter\noexpand\csname#1\endcsname} % Hyphenation fixes. \hyphenation{ Flor-i-da Ghost-script Ghost-view Mac-OS Post-Script ap-pen-dix bit-map bit-maps data-base data-bases eshell fall-ing half-way long-est man-u-script man-u-scripts mini-buf-fer mini-buf-fers over-view par-a-digm par-a-digms rath-er rec-tan-gu-lar ro-bot-ics se-vere-ly set-up spa-ces spell-ing spell-ings stand-alone strong-est time-stamp time-stamps which-ever white-space wide-spread wrap-around } % Sometimes it is convenient to have everything in the transcript file % and nothing on the terminal. We don't just call \tracingall here, % since that produces some useless output on the terminal. We also make % some effort to order the tracing commands to reduce output in the log % file; cf. trace.sty in LaTeX. % \def\gloggingall{\begingroup \globaldefs = 1 \loggingall \endgroup}% \def\loggingall{% \tracingstats2 \tracingpages1 \tracinglostchars2 % 2 gives us more in etex \tracingparagraphs1 \tracingoutput1 \tracingmacros2 \tracingrestores1 \showboxbreadth\maxdimen \showboxdepth\maxdimen \ifx\eTeXversion\thisisundefined\else % etex gives us more logging \tracingscantokens1 \tracingifs1 \tracinggroups1 \tracingnesting2 \tracingassigns1 \fi \tracingcommands3 % 3 gives us more in etex \errorcontextlines16 }% % @errormsg{MSG}. Do the index-like expansions on MSG, but if things % aren't perfect, it's not the end of the world, being an error message, % after all. % \def\errormsg{\begingroup \indexnofonts \doerrormsg} \def\doerrormsg#1{\errmessage{#1}} % add check for \lastpenalty to plain's definitions. If the last thing % we did was a \nobreak, we don't want to insert more space. % \def\smallbreak{\ifnum\lastpenalty<10000\par\ifdim\lastskip<\smallskipamount \removelastskip\penalty-50\smallskip\fi\fi} \def\medbreak{\ifnum\lastpenalty<10000\par\ifdim\lastskip<\medskipamount \removelastskip\penalty-100\medskip\fi\fi} \def\bigbreak{\ifnum\lastpenalty<10000\par\ifdim\lastskip<\bigskipamount \removelastskip\penalty-200\bigskip\fi\fi} % Output routine % % For a final copy, take out the rectangles % that mark overfull boxes (in case you have decided % that the text looks ok even though it passes the margin). % \def\finalout{\overfullrule=0pt } % Do @cropmarks to get crop marks. % \newif\ifcropmarks \let\cropmarks = \cropmarkstrue % % Dimensions to add cropmarks at corners. % Added by P. A. MacKay, 12 Nov. 1986 % \newdimen\outerhsize \newdimen\outervsize % set by the paper size routines \newdimen\cornerlong \cornerlong=1pc \newdimen\cornerthick \cornerthick=.3pt \newdimen\topandbottommargin \topandbottommargin=.75in % Output a mark which sets \thischapter, \thissection and \thiscolor. % We dump everything together because we only have one kind of mark. % This works because we only use \botmark / \topmark, not \firstmark. % % A mark contains a subexpression of the \ifcase ... \fi construct. % \get*marks macros below extract the needed part using \ifcase. % % Another complication is to let the user choose whether \thischapter % (\thissection) refers to the chapter (section) in effect at the top % of a page, or that at the bottom of a page. % \domark is called twice inside \chapmacro, to add one % mark before the section break, and one after. % In the second call \prevchapterdefs is the same as \lastchapterdefs, % and \prevsectiondefs is the same as \lastsectiondefs. % Then if the page is not broken at the mark, some of the previous % section appears on the page, and we can get the name of this section % from \firstmark for @everyheadingmarks top. % @everyheadingmarks bottom uses \botmark. % % See page 260 of The TeXbook. \def\domark{% \toks0=\expandafter{\lastchapterdefs}% \toks2=\expandafter{\lastsectiondefs}% \toks4=\expandafter{\prevchapterdefs}% \toks6=\expandafter{\prevsectiondefs}% \toks8=\expandafter{\lastcolordefs}% \mark{% \the\toks0 \the\toks2 % 0: marks for @everyheadingmarks top \noexpand\or \the\toks4 \the\toks6 % 1: for @everyheadingmarks bottom \noexpand\else \the\toks8 % 2: color marks }% } % \gettopheadingmarks, \getbottomheadingmarks, % \getcolormarks - extract needed part of mark. % % \topmark doesn't work for the very first chapter (after the title % page or the contents), so we use \firstmark there -- this gets us % the mark with the chapter defs, unless the user sneaks in, e.g., % @setcolor (or @url, or @link, etc.) between @contents and the very % first @chapter. \def\gettopheadingmarks{% \ifcase0\topmark\fi \ifx\thischapter\empty \ifcase0\firstmark\fi \fi } \def\getbottomheadingmarks{\ifcase1\botmark\fi} \def\getcolormarks{\ifcase2\topmark\fi} % Avoid "undefined control sequence" errors. \def\lastchapterdefs{} \def\lastsectiondefs{} \def\lastsection{} \def\prevchapterdefs{} \def\prevsectiondefs{} \def\lastcolordefs{} % Margin to add to right of even pages, to left of odd pages. \newdimen\bindingoffset \newdimen\normaloffset \newdimen\txipagewidth \newdimen\txipageheight % Main output routine. % \chardef\PAGE = 255 \output = {\onepageout{\pagecontents\PAGE}} \newbox\headlinebox \newbox\footlinebox % \onepageout takes a vbox as an argument. % \shipout a vbox for a single page, adding an optional header, footer, % cropmarks, and footnote. This also causes index entries for this page % to be written to the auxiliary files. % \def\onepageout#1{% \ifcropmarks \hoffset=0pt \else \hoffset=\normaloffset \fi % \ifodd\pageno \advance\hoffset by \bindingoffset \else \advance\hoffset by -\bindingoffset\fi % % Common context changes for both heading and footing. % Do this outside of the \shipout so @code etc. will be expanded in % the headline as they should be, not taken literally (outputting ''code). \def\commmonheadfootline{\let\hsize=\txipagewidth \texinfochars} % % Retrieve the information for the headings from the marks in the page, % and call Plain TeX's \makeheadline and \makefootline, which use the % values in \headline and \footline. % % This is used to check if we are on the first page of a chapter. \ifcase1\topmark\fi \let\prevchaptername\thischaptername \ifcase0\firstmark\fi \let\curchaptername\thischaptername % \ifodd\pageno \getoddheadingmarks \else \getevenheadingmarks \fi \ifodd\pageno \getoddfootingmarks \else \getevenfootingmarks \fi % \ifx\curchaptername\prevchaptername \let\thischapterheading\thischapter \else % \thischapterheading is the same as \thischapter except it is blank % for the first page of a chapter. This is to prevent the chapter name % being shown twice. \def\thischapterheading{}% \fi % \global\setbox\headlinebox = \vbox{\commmonheadfootline \makeheadline}% \global\setbox\footlinebox = \vbox{\commmonheadfootline \makefootline}% % {% % Set context for writing to auxiliary files like index files. % Have to do this stuff outside the \shipout because we want it to % take effect in \write's, yet the group defined by the \vbox ends % before the \shipout runs. % \indexdummies % don't expand commands in the output. \normalturnoffactive % \ in index entries must not stay \, e.g., if % the page break happens to be in the middle of an example. % We don't want .vr (or whatever) entries like this: % \entry{{\indexbackslash }acronym}{32}{\code {\acronym}} % "\acronym" won't work when it's read back in; % it needs to be % {\code {{\backslashcurfont }acronym} \shipout\vbox{% % Do this early so pdf references go to the beginning of the page. \ifpdfmakepagedest \pdfdest name{\the\pageno} xyz\fi % \ifcropmarks \vbox to \outervsize\bgroup \hsize = \outerhsize \vskip-\topandbottommargin \vtop to0pt{% \line{\ewtop\hfil\ewtop}% \nointerlineskip \line{% \vbox{\moveleft\cornerthick\nstop}% \hfill \vbox{\moveright\cornerthick\nstop}% }% \vss}% \vskip\topandbottommargin \line\bgroup \hfil % center the page within the outer (page) hsize. \ifodd\pageno\hskip\bindingoffset\fi \vbox\bgroup \fi % \unvbox\headlinebox \pagebody{#1}% \ifdim\ht\footlinebox > 0pt % Only leave this space if the footline is nonempty. % (We lessened \vsize for it in \oddfootingyyy.) % The \baselineskip=24pt in plain's \makefootline has no effect. \vskip 24pt \unvbox\footlinebox \fi % \ifcropmarks \egroup % end of \vbox\bgroup \hfil\egroup % end of (centering) \line\bgroup \vskip\topandbottommargin plus1fill minus1fill \boxmaxdepth = \cornerthick \vbox to0pt{\vss \line{% \vbox{\moveleft\cornerthick\nsbot}% \hfill \vbox{\moveright\cornerthick\nsbot}% }% \nointerlineskip \line{\ewbot\hfil\ewbot}% }% \egroup % \vbox from first cropmarks clause \fi }% end of \shipout\vbox }% end of group with \indexdummies \advancepageno \ifnum\outputpenalty>-20000 \else\dosupereject\fi } \newinsert\margin \dimen\margin=\maxdimen % Main part of page, including any footnotes \def\pagebody#1{\vbox to\txipageheight{\boxmaxdepth=\maxdepth #1}} {\catcode`\@ =11 \gdef\pagecontents#1{\ifvoid\topins\else\unvbox\topins\fi % marginal hacks, juha@viisa.uucp (Juha Takala) \ifvoid\margin\else % marginal info is present \rlap{\kern\hsize\vbox to\z@{\kern1pt\box\margin \vss}}\fi \dimen@=\dp#1\relax \unvbox#1\relax \ifvoid\footins\else\vskip\skip\footins\footnoterule \unvbox\footins\fi \ifr@ggedbottom \kern-\dimen@ \vfil \fi} } % Here are the rules for the cropmarks. Note that they are % offset so that the space between them is truly \outerhsize or \outervsize % (P. A. MacKay, 12 November, 1986) % \def\ewtop{\vrule height\cornerthick depth0pt width\cornerlong} \def\nstop{\vbox {\hrule height\cornerthick depth\cornerlong width\cornerthick}} \def\ewbot{\vrule height0pt depth\cornerthick width\cornerlong} \def\nsbot{\vbox {\hrule height\cornerlong depth\cornerthick width\cornerthick}} % Argument parsing % Parse an argument, then pass it to #1. The argument is the rest of % the input line (except we remove a trailing comment). #1 should be a % macro which expects an ordinary undelimited TeX argument. % For example, \def\foo{\parsearg\fooxxx}. % \def\parsearg{\parseargusing{}} \def\parseargusing#1#2{% \def\argtorun{#2}% \begingroup \obeylines \spaceisspace #1% \parseargline\empty% Insert the \empty token, see \finishparsearg below. } {\obeylines % \gdef\parseargline#1^^M{% \endgroup % End of the group started in \parsearg. \argremovecomment #1\comment\ArgTerm% }% } % First remove any @comment, then any @c comment. Also remove a @texinfoc % comment (see \scanmacro for details). Pass the result on to \argcheckspaces. \def\argremovecomment#1\comment#2\ArgTerm{\argremovec #1\c\ArgTerm} \def\argremovec#1\c#2\ArgTerm{\argremovetexinfoc #1\texinfoc\ArgTerm} \def\argremovetexinfoc#1\texinfoc#2\ArgTerm{\argcheckspaces#1\^^M\ArgTerm} % Each occurrence of `\^^M' or `<space>\^^M' is replaced by a single space. % % \argremovec might leave us with trailing space, e.g., % @end itemize @c foo % This space token undergoes the same procedure and is eventually removed % by \finishparsearg. % \def\argcheckspaces#1\^^M{\argcheckspacesX#1\^^M \^^M} \def\argcheckspacesX#1 \^^M{\argcheckspacesY#1\^^M} \def\argcheckspacesY#1\^^M#2\^^M#3\ArgTerm{% \def\temp{#3}% \ifx\temp\empty % Do not use \next, perhaps the caller of \parsearg uses it; reuse \temp: \let\temp\finishparsearg \else \let\temp\argcheckspaces \fi % Put the space token in: \temp#1 #3\ArgTerm } % If a _delimited_ argument is enclosed in braces, they get stripped; so % to get _exactly_ the rest of the line, we had to prevent such situation. % We prepended an \empty token at the very beginning and we expand it now, % just before passing the control to \argtorun. % (Similarly, we have to think about #3 of \argcheckspacesY above: it is % either the null string, or it ends with \^^M---thus there is no danger % that a pair of braces would be stripped. % % But first, we have to remove the trailing space token. % \def\finishparsearg#1 \ArgTerm{\expandafter\argtorun\expandafter{#1}} % \parseargdef - define a command taking an argument on the line % % \parseargdef\foo{...} % is roughly equivalent to % \def\foo{\parsearg\Xfoo} % \def\Xfoo#1{...} \def\parseargdef#1{% \expandafter \doparseargdef \csname\string#1\endcsname #1% } \def\doparseargdef#1#2{% \def#2{\parsearg#1}% \def#1##1% } % Several utility definitions with active space: { \obeyspaces \gdef\obeyedspace{ } % Make each space character in the input produce a normal interword % space in the output. Don't allow a line break at this space, as this % is used only in environments like @example, where each line of input % should produce a line of output anyway. % \gdef\sepspaces{\obeyspaces\let =\tie} % If an index command is used in an @example environment, any spaces % therein should become regular spaces in the raw index file, not the % expansion of \tie (\leavevmode \penalty \@M \ ). \gdef\unsepspaces{\let =\space} } \def\flushcr{\ifx\par\lisppar \def\next##1{}\else \let\next=\relax \fi \next} % Define the framework for environments in texinfo.tex. It's used like this: % % \envdef\foo{...} % \def\Efoo{...} % % It's the responsibility of \envdef to insert \begingroup before the % actual body; @end closes the group after calling \Efoo. \envdef also % defines \thisenv, so the current environment is known; @end checks % whether the environment name matches. The \checkenv macro can also be % used to check whether the current environment is the one expected. % % Non-false conditionals (@iftex, @ifset) don't fit into this, so they % are not treated as environments; they don't open a group. (The % implementation of @end takes care not to call \endgroup in this % special case.) % At run-time, environments start with this: \def\startenvironment#1{\begingroup\def\thisenv{#1}} % initialize \let\thisenv\empty % ... but they get defined via ``\envdef\foo{...}'': \long\def\envdef#1#2{\def#1{\startenvironment#1#2}} \def\envparseargdef#1#2{\parseargdef#1{\startenvironment#1#2}} % Check whether we're in the right environment: \def\checkenv#1{% \def\temp{#1}% \ifx\thisenv\temp \else \badenverr \fi } % Environment mismatch, #1 expected: \def\badenverr{% \errhelp = \EMsimple \errmessage{This command can appear only \inenvironment\temp, not \inenvironment\thisenv}% } \def\inenvironment#1{% \ifx#1\empty outside of any environment% \else in environment \expandafter\string#1% \fi } % @end foo executes the definition of \Efoo. % But first, it executes a specialized version of \checkenv % \parseargdef\end{% \if 1\csname iscond.#1\endcsname \else % The general wording of \badenverr may not be ideal. \expandafter\checkenv\csname#1\endcsname \csname E#1\endcsname \endgroup \fi } \newhelp\EMsimple{Press RETURN to continue.} % Be sure we're in horizontal mode when doing a tie, since we make space % equivalent to this in @example-like environments. Otherwise, a space % at the beginning of a line will start with \penalty -- and % since \penalty is valid in vertical mode, we'd end up putting the % penalty on the vertical list instead of in the new paragraph. {\catcode`@ = 11 % Avoid using \@M directly, because that causes trouble % if the definition is written into an index file. \global\let\tiepenalty = \@M \gdef\tie{\leavevmode\penalty\tiepenalty\ } } % @: forces normal size whitespace following. \def\:{\spacefactor=1000 } % @* forces a line break. \def\*{\unskip\hfil\break\hbox{}\ignorespaces} % @/ allows a line break. \let\/=\allowbreak % @. is an end-of-sentence period. \def\.{.\spacefactor=\endofsentencespacefactor\space} % @! is an end-of-sentence bang. \def\!{!\spacefactor=\endofsentencespacefactor\space} % @? is an end-of-sentence query. \def\?{?\spacefactor=\endofsentencespacefactor\space} % @frenchspacing on|off says whether to put extra space after punctuation. % \def\onword{on} \def\offword{off} % \parseargdef\frenchspacing{% \def\temp{#1}% \ifx\temp\onword \plainfrenchspacing \else\ifx\temp\offword \plainnonfrenchspacing \else \errhelp = \EMsimple \errmessage{Unknown @frenchspacing option `\temp', must be on|off}% \fi\fi } % @w prevents a word break. Without the \leavevmode, @w at the % beginning of a paragraph, when TeX is still in vertical mode, would % produce a whole line of output instead of starting the paragraph. \def\w#1{\leavevmode\hbox{#1}} % @group ... @end group forces ... to be all on one page, by enclosing % it in a TeX vbox. We use \vtop instead of \vbox to construct the box % to keep its height that of a normal line. According to the rules for % \topskip (p.114 of the TeXbook), the glue inserted is % max (\topskip - \ht (first item), 0). If that height is large, % therefore, no glue is inserted, and the space between the headline and % the text is small, which looks bad. % % Another complication is that the group might be very large. This can % cause the glue on the previous page to be unduly stretched, because it % does not have much material. In this case, it's better to add an % explicit \vfill so that the extra space is at the bottom. The % threshold for doing this is if the group is more than \vfilllimit % percent of a page (\vfilllimit can be changed inside of @tex). % \newbox\groupbox \def\vfilllimit{0.7} % \envdef\group{% \ifnum\catcode`\^^M=\active \else \errhelp = \groupinvalidhelp \errmessage{@group invalid in context where filling is enabled}% \fi \startsavinginserts % \setbox\groupbox = \vtop\bgroup % Do @comment since we are called inside an environment such as % @example, where each end-of-line in the input causes an % end-of-line in the output. We don't want the end-of-line after % the `@group' to put extra space in the output. Since @group % should appear on a line by itself (according to the Texinfo % manual), we don't worry about eating any user text. \comment } % % The \vtop produces a box with normal height and large depth; thus, TeX puts % \baselineskip glue before it, and (when the next line of text is done) % \lineskip glue after it. Thus, space below is not quite equal to space % above. But it's pretty close. \def\Egroup{% % To get correct interline space between the last line of the group % and the first line afterwards, we have to propagate \prevdepth. \endgraf % Not \par, as it may have been set to \lisppar. \global\dimen1 = \prevdepth \egroup % End the \vtop. \addgroupbox \prevdepth = \dimen1 \checkinserts } \def\addgroupbox{ % \dimen0 is the vertical size of the group's box. \dimen0 = \ht\groupbox \advance\dimen0 by \dp\groupbox % \dimen2 is how much space is left on the page (more or less). \dimen2 = \txipageheight \advance\dimen2 by -\pagetotal % if the group doesn't fit on the current page, and it's a big big % group, force a page break. \ifdim \dimen0 > \dimen2 \ifdim \pagetotal < \vfilllimit\txipageheight \page \fi \fi \box\groupbox } % % TeX puts in an \escapechar (i.e., `@') at the beginning of the help % message, so this ends up printing `@group can only ...'. % \newhelp\groupinvalidhelp{% group can only be used in environments such as @example,^^J% where each line of input produces a line of output.} % @need space-in-mils % forces a page break if there is not space-in-mils remaining. \newdimen\mil \mil=0.001in \parseargdef\need{% % Ensure vertical mode, so we don't make a big box in the middle of a % paragraph. \par % % If the @need value is less than one line space, it's useless. \dimen0 = #1\mil \dimen2 = \ht\strutbox \advance\dimen2 by \dp\strutbox \ifdim\dimen0 > \dimen2 % % Do a \strut just to make the height of this box be normal, so the % normal leading is inserted relative to the preceding line. % And a page break here is fine. \vtop to #1\mil{\strut\vfil}% % % TeX does not even consider page breaks if a penalty added to the % main vertical list is 10000 or more. But in order to see if the % empty box we just added fits on the page, we must make it consider % page breaks. On the other hand, we don't want to actually break the % page after the empty box. So we use a penalty of 9999. % % There is an extremely small chance that TeX will actually break the % page at this \penalty, if there are no other feasible breakpoints in % sight. (If the user is using lots of big @group commands, which % almost-but-not-quite fill up a page, TeX will have a hard time doing % good page breaking, for example.) However, I could not construct an % example where a page broke at this \penalty; if it happens in a real % document, then we can reconsider our strategy. \penalty9999 % % Back up by the size of the box, whether we did a page break or not. \kern -#1\mil % % Do not allow a page break right after this kern. \nobreak \fi } % @br forces paragraph break (and is undocumented). \let\br = \par % @page forces the start of a new page. % \def\page{\par\vfill\supereject} % @exdent text.... % outputs text on separate line in roman font, starting at standard page margin % This records the amount of indent in the innermost environment. % That's how much \exdent should take out. \newskip\exdentamount % This defn is used inside fill environments such as @defun. \parseargdef\exdent{\hfil\break\hbox{\kern -\exdentamount{\rm#1}}\hfil\break} % This defn is used inside nofill environments such as @example. \parseargdef\nofillexdent{{\advance \leftskip by -\exdentamount \leftline{\hskip\leftskip{\rm#1}}}} % @inmargin{WHICH}{TEXT} puts TEXT in the WHICH margin next to the current % paragraph. For more general purposes, use the \margin insertion % class. WHICH is `l' or `r'. Not documented, written for gawk manual. % \newskip\inmarginspacing \inmarginspacing=1cm \def\strutdepth{\dp\strutbox} % \def\doinmargin#1#2{\strut\vadjust{% \nobreak \kern-\strutdepth \vtop to \strutdepth{% \baselineskip=\strutdepth \vss % if you have multiple lines of stuff to put here, you'll need to % make the vbox yourself of the appropriate size. \ifx#1l% \llap{\ignorespaces #2\hskip\inmarginspacing}% \else \rlap{\hskip\hsize \hskip\inmarginspacing \ignorespaces #2}% \fi \null }% }} \def\inleftmargin{\doinmargin l} \def\inrightmargin{\doinmargin r} % % @inmargin{TEXT [, RIGHT-TEXT]} % (if RIGHT-TEXT is given, use TEXT for left page, RIGHT-TEXT for right; % else use TEXT for both). % \def\inmargin#1{\parseinmargin #1,,\finish} \def\parseinmargin#1,#2,#3\finish{% not perfect, but better than nothing. \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0 > 0pt \def\lefttext{#1}% have both texts \def\righttext{#2}% \else \def\lefttext{#1}% have only one text \def\righttext{#1}% \fi % \ifodd\pageno \def\temp{\inrightmargin\righttext}% odd page -> outside is right margin \else \def\temp{\inleftmargin\lefttext}% \fi \temp } % @include FILE -- \input text of FILE. % \def\include{\parseargusing\filenamecatcodes\includezzz} \def\includezzz#1{% \pushthisfilestack \def\thisfile{#1}% {% \makevalueexpandable % we want to expand any @value in FILE. \turnoffactive % and allow special characters in the expansion \indexnofonts % Allow `@@' and other weird things in file names. \wlog{texinfo.tex: doing @include of #1^^J}% \edef\temp{\noexpand\input #1 }% % % This trickery is to read FILE outside of a group, in case it makes % definitions, etc. \expandafter }\temp \popthisfilestack } \def\filenamecatcodes{% \catcode`\\=\other \catcode`~=\other \catcode`^=\other \catcode`_=\other \catcode`|=\other \catcode`<=\other \catcode`>=\other \catcode`+=\other \catcode`-=\other \catcode`\`=\other \catcode`\'=\other } \def\pushthisfilestack{% \expandafter\pushthisfilestackX\popthisfilestack\StackTerm } \def\pushthisfilestackX{% \expandafter\pushthisfilestackY\thisfile\StackTerm } \def\pushthisfilestackY #1\StackTerm #2\StackTerm {% \gdef\popthisfilestack{\gdef\thisfile{#1}\gdef\popthisfilestack{#2}}% } \def\popthisfilestack{\errthisfilestackempty} \def\errthisfilestackempty{\errmessage{Internal error: the stack of filenames is empty.}} % \def\thisfile{} % @center line % outputs that line, centered. % \parseargdef\center{% \ifhmode \let\centersub\centerH \else \let\centersub\centerV \fi \centersub{\hfil \ignorespaces#1\unskip \hfil}% \let\centersub\relax % don't let the definition persist, just in case } \def\centerH#1{{% \hfil\break \advance\hsize by -\leftskip \advance\hsize by -\rightskip \line{#1}% \break }} % \newcount\centerpenalty \def\centerV#1{% % The idea here is the same as in \startdefun, \cartouche, etc.: if % @center is the first thing after a section heading, we need to wipe % out the negative parskip inserted by \sectionheading, but still % prevent a page break here. \centerpenalty = \lastpenalty \ifnum\centerpenalty>10000 \vskip\parskip \fi \ifnum\centerpenalty>9999 \penalty\centerpenalty \fi \line{\kern\leftskip #1\kern\rightskip}% } % @sp n outputs n lines of vertical space % \parseargdef\sp{\vskip #1\baselineskip} % @comment ...line which is ignored... % @c is the same as @comment % @ignore ... @end ignore is another way to write a comment \def\c{\begingroup \catcode`\^^M=\active% \catcode`\@=\other \catcode`\{=\other \catcode`\}=\other% \cxxx} {\catcode`\^^M=\active \gdef\cxxx#1^^M{\endgroup}} % \let\comment\c % @paragraphindent NCHARS % We'll use ems for NCHARS, close enough. % NCHARS can also be the word `asis' or `none'. % We cannot feasibly implement @paragraphindent asis, though. % \def\asisword{asis} % no translation, these are keywords \def\noneword{none} % \parseargdef\paragraphindent{% \def\temp{#1}% \ifx\temp\asisword \else \ifx\temp\noneword \defaultparindent = 0pt \else \defaultparindent = #1em \fi \fi \parindent = \defaultparindent } % @exampleindent NCHARS % We'll use ems for NCHARS like @paragraphindent. % It seems @exampleindent asis isn't necessary, but % I preserve it to make it similar to @paragraphindent. \parseargdef\exampleindent{% \def\temp{#1}% \ifx\temp\asisword \else \ifx\temp\noneword \lispnarrowing = 0pt \else \lispnarrowing = #1em \fi \fi } % @firstparagraphindent WORD % If WORD is `none', then suppress indentation of the first paragraph % after a section heading. If WORD is `insert', then do indent at such % paragraphs. % % The paragraph indentation is suppressed or not by calling % \suppressfirstparagraphindent, which the sectioning commands do. % We switch the definition of this back and forth according to WORD. % By default, we suppress indentation. % \def\suppressfirstparagraphindent{\dosuppressfirstparagraphindent} \def\insertword{insert} % \parseargdef\firstparagraphindent{% \def\temp{#1}% \ifx\temp\noneword \let\suppressfirstparagraphindent = \dosuppressfirstparagraphindent \else\ifx\temp\insertword \let\suppressfirstparagraphindent = \relax \else \errhelp = \EMsimple \errmessage{Unknown @firstparagraphindent option `\temp'}% \fi\fi } % Here is how we actually suppress indentation. Redefine \everypar to % \kern backwards by \parindent, and then reset itself to empty. % % We also make \indent itself not actually do anything until the next % paragraph. % \gdef\dosuppressfirstparagraphindent{% \gdef\indent {\restorefirstparagraphindent \indent}% \gdef\noindent{\restorefirstparagraphindent \noindent}% \global\everypar = {\kern -\parindent \restorefirstparagraphindent}% } % \gdef\restorefirstparagraphindent{% \global\let\indent = \ptexindent \global\let\noindent = \ptexnoindent \global\everypar = {}% } % @refill is a no-op. \let\refill=\relax % @setfilename INFO-FILENAME - ignored \let\setfilename=\comment % @bye. \outer\def\bye{\pagealignmacro\tracingstats=1\ptexend} \message{pdf,} % adobe `portable' document format \newcount\tempnum \newcount\lnkcount \newtoks\filename \newcount\filenamelength \newcount\pgn \newtoks\toksA \newtoks\toksB \newtoks\toksC \newtoks\toksD \newbox\boxA \newbox\boxB \newcount\countA \newif\ifpdf \newif\ifpdfmakepagedest % % For LuaTeX % \newif\iftxiuseunicodedestname \txiuseunicodedestnamefalse % For pdfTeX etc. \ifx\luatexversion\thisisundefined \else % Use Unicode destination names \txiuseunicodedestnametrue % Escape PDF strings with converting UTF-16 from UTF-8 \begingroup \catcode`\%=12 \directlua{ function UTF16oct(str) tex.sprint(string.char(0x5c) .. '376' .. string.char(0x5c) .. '377') for c in string.utfvalues(str) do if c < 0x10000 then tex.sprint( string.format(string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o', (c / 256), (c % 256))) else c = c - 0x10000 local c_hi = c / 1024 + 0xd800 local c_lo = c % 1024 + 0xdc00 tex.sprint( string.format(string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o' .. string.char(0x5c) .. string.char(0x25) .. '03o', (c_hi / 256), (c_hi % 256), (c_lo / 256), (c_lo % 256))) end end end } \endgroup \def\pdfescapestrutfsixteen#1{\directlua{UTF16oct('\luaescapestring{#1}')}} % Escape PDF strings without converting \begingroup \directlua{ function PDFescstr(str) for c in string.bytes(str) do if c <= 0x20 or c >= 0x80 or c == 0x28 or c == 0x29 or c == 0x5c then tex.sprint( string.format(string.char(0x5c) .. string.char(0x25) .. '03o', c)) else tex.sprint(string.char(c)) end end end } \endgroup \def\pdfescapestring#1{\directlua{PDFescstr('\luaescapestring{#1}')}} \ifnum\luatexversion>84 % For LuaTeX >= 0.85 \def\pdfdest{\pdfextension dest} \let\pdfoutput\outputmode \def\pdfliteral{\pdfextension literal} \def\pdfcatalog{\pdfextension catalog} \def\pdftexversion{\numexpr\pdffeedback version\relax} \let\pdfximage\saveimageresource \let\pdfrefximage\useimageresource \let\pdflastximage\lastsavedimageresourceindex \def\pdfendlink{\pdfextension endlink\relax} \def\pdfoutline{\pdfextension outline} \def\pdfstartlink{\pdfextension startlink} \def\pdffontattr{\pdfextension fontattr} \def\pdfobj{\pdfextension obj} \def\pdflastobj{\numexpr\pdffeedback lastobj\relax} \let\pdfpagewidth\pagewidth \let\pdfpageheight\pageheight \edef\pdfhorigin{\pdfvariable horigin} \edef\pdfvorigin{\pdfvariable vorigin} \fi \fi % when pdftex is run in dvi mode, \pdfoutput is defined (so \pdfoutput=1 % can be set). So we test for \relax and 0 as well as being undefined. \ifx\pdfoutput\thisisundefined \else \ifx\pdfoutput\relax \else \ifcase\pdfoutput \else \pdftrue \fi \fi \fi % PDF uses PostScript string constants for the names of xref targets, % for display in the outlines, and in other places. Thus, we have to % double any backslashes. Otherwise, a name like "\node" will be % interpreted as a newline (\n), followed by o, d, e. Not good. % % See http://www.ntg.nl/pipermail/ntg-pdftex/2004-July/000654.html and % related messages. The final outcome is that it is up to the TeX user % to double the backslashes and otherwise make the string valid, so % that's what we do. pdftex 1.30.0 (ca.2005) introduced a primitive to % do this reliably, so we use it. % #1 is a control sequence in which to do the replacements, % which we \xdef. \def\txiescapepdf#1{% \ifx\pdfescapestring\thisisundefined % No primitive available; should we give a warning or log? % Many times it won't matter. \xdef#1{#1}% \else % The expandable \pdfescapestring primitive escapes parentheses, % backslashes, and other special chars. \xdef#1{\pdfescapestring{#1}}% \fi } \def\txiescapepdfutfsixteen#1{% \ifx\pdfescapestrutfsixteen\thisisundefined % No UTF-16 converting macro available. \txiescapepdf{#1}% \else \xdef#1{\pdfescapestrutfsixteen{#1}}% \fi } \newhelp\nopdfimagehelp{Texinfo supports .png, .jpg, .jpeg, and .pdf images with PDF output, and none of those formats could be found. (.eps cannot be supported due to the design of the PDF format; use regular TeX (DVI output) for that.)} \ifpdf % % Color manipulation macros using ideas from pdfcolor.tex, % except using rgb instead of cmyk; the latter is said to render as a % very dark gray on-screen and a very dark halftone in print, instead % of actual black. The dark red here is dark enough to print on paper as % nearly black, but still distinguishable for online viewing. We use % black by default, though. \def\rgbDarkRed{0.50 0.09 0.12} \def\rgbBlack{0 0 0} % % rg sets the color for filling (usual text, etc.); % RG sets the color for stroking (thin rules, e.g., normal _'s). \def\pdfsetcolor#1{\pdfliteral{#1 rg #1 RG}} % % Set color, and create a mark which defines \thiscolor accordingly, % so that \makeheadline knows which color to restore. \def\setcolor#1{% \xdef\lastcolordefs{\gdef\noexpand\thiscolor{#1}}% \domark \pdfsetcolor{#1}% } % \def\maincolor{\rgbBlack} \pdfsetcolor{\maincolor} \edef\thiscolor{\maincolor} \def\lastcolordefs{} % \def\makefootline{% \baselineskip24pt \line{\pdfsetcolor{\maincolor}\the\footline}% } % \def\makeheadline{% \vbox to 0pt{% \vskip-22.5pt \line{% \vbox to8.5pt{}% % Extract \thiscolor definition from the marks. \getcolormarks % Typeset the headline with \maincolor, then restore the color. \pdfsetcolor{\maincolor}\the\headline\pdfsetcolor{\thiscolor}% }% \vss }% \nointerlineskip } % % \pdfcatalog{/PageMode /UseOutlines} % % #1 is image name, #2 width (might be empty/whitespace), #3 height (ditto). \def\dopdfimage#1#2#3{% \def\pdfimagewidth{#2}\setbox0 = \hbox{\ignorespaces #2}% \def\pdfimageheight{#3}\setbox2 = \hbox{\ignorespaces #3}% % % pdftex (and the PDF format) support .pdf, .png, .jpg (among % others). Let's try in that order, PDF first since if % someone has a scalable image, presumably better to use that than a % bitmap. \let\pdfimgext=\empty \begingroup \openin 1 #1.pdf \ifeof 1 \openin 1 #1.PDF \ifeof 1 \openin 1 #1.png \ifeof 1 \openin 1 #1.jpg \ifeof 1 \openin 1 #1.jpeg \ifeof 1 \openin 1 #1.JPG \ifeof 1 \errhelp = \nopdfimagehelp \errmessage{Could not find image file #1 for pdf}% \else \gdef\pdfimgext{JPG}% \fi \else \gdef\pdfimgext{jpeg}% \fi \else \gdef\pdfimgext{jpg}% \fi \else \gdef\pdfimgext{png}% \fi \else \gdef\pdfimgext{PDF}% \fi \else \gdef\pdfimgext{pdf}% \fi \closein 1 \endgroup % % without \immediate, ancient pdftex seg faults when the same image is % included twice. (Version 3.14159-pre-1.0-unofficial-20010704.) \ifnum\pdftexversion < 14 \immediate\pdfimage \else \immediate\pdfximage \fi \ifdim \wd0 >0pt width \pdfimagewidth \fi \ifdim \wd2 >0pt height \pdfimageheight \fi \ifnum\pdftexversion<13 #1.\pdfimgext \else {#1.\pdfimgext}% \fi \ifnum\pdftexversion < 14 \else \pdfrefximage \pdflastximage \fi} % \def\setpdfdestname#1{{% % We have to set dummies so commands such as @code, and characters % such as \, aren't expanded when present in a section title. \indexnofonts \makevalueexpandable \turnoffactive \iftxiuseunicodedestname \ifx \declaredencoding \latone % Pass through Latin-1 characters. % LuaTeX with byte wise I/O converts Latin-1 characters to Unicode. \else \ifx \declaredencoding \utfeight % Pass through Unicode characters. \else % Use ASCII approximations in destination names. \passthroughcharsfalse \fi \fi \else % Use ASCII approximations in destination names. \passthroughcharsfalse \fi \def\pdfdestname{#1}% \txiescapepdf\pdfdestname }} % \def\setpdfoutlinetext#1{{% \indexnofonts \makevalueexpandable \turnoffactive \ifx \declaredencoding \latone % The PDF format can use an extended form of Latin-1 in bookmark % strings. See Appendix D of the PDF Reference, Sixth Edition, for % the "PDFDocEncoding". \passthroughcharstrue % Pass through Latin-1 characters. % LuaTeX: Convert to Unicode % pdfTeX: Use Latin-1 as PDFDocEncoding \def\pdfoutlinetext{#1}% \else \ifx \declaredencoding \utfeight \ifx\luatexversion\thisisundefined % For pdfTeX with UTF-8. % TODO: the PDF format can use UTF-16 in bookmark strings, % but the code for this isn't done yet. % Use ASCII approximations. \passthroughcharsfalse \def\pdfoutlinetext{#1}% \else % For LuaTeX with UTF-8. % Pass through Unicode characters for title texts. \passthroughcharstrue \def\pdfoutlinetext{#1}% \fi \else % For non-Latin-1 or non-UTF-8 encodings. % Use ASCII approximations. \passthroughcharsfalse \def\pdfoutlinetext{#1}% \fi \fi % LuaTeX: Convert to UTF-16 % pdfTeX: Use Latin-1 as PDFDocEncoding \txiescapepdfutfsixteen\pdfoutlinetext }} % \def\pdfmkdest#1{% \setpdfdestname{#1}% \safewhatsit{\pdfdest name{\pdfdestname} xyz}% } % % used to mark target names; must be expandable. \def\pdfmkpgn#1{#1} % % by default, use black for everything. \def\urlcolor{\rgbBlack} \def\linkcolor{\rgbBlack} \def\endlink{\setcolor{\maincolor}\pdfendlink} % % Adding outlines to PDF; macros for calculating structure of outlines % come from Petr Olsak \def\expnumber#1{\expandafter\ifx\csname#1\endcsname\relax 0% \else \csname#1\endcsname \fi} \def\advancenumber#1{\tempnum=\expnumber{#1}\relax \advance\tempnum by 1 \expandafter\xdef\csname#1\endcsname{\the\tempnum}} % % #1 is the section text, which is what will be displayed in the % outline by the pdf viewer. #2 is the pdf expression for the number % of subentries (or empty, for subsubsections). #3 is the node text, % which might be empty if this toc entry had no corresponding node. % #4 is the page number % \def\dopdfoutline#1#2#3#4{% % Generate a link to the node text if that exists; else, use the % page number. We could generate a destination for the section % text in the case where a section has no node, but it doesn't % seem worth the trouble, since most documents are normally structured. \setpdfoutlinetext{#1} \setpdfdestname{#3} \ifx\pdfdestname\empty \def\pdfdestname{#4}% \fi % \pdfoutline goto name{\pdfmkpgn{\pdfdestname}}#2{\pdfoutlinetext}% } % \def\pdfmakeoutlines{% \begingroup % Read toc silently, to get counts of subentries for \pdfoutline. \def\partentry##1##2##3##4{}% ignore parts in the outlines \def\numchapentry##1##2##3##4{% \def\thischapnum{##2}% \def\thissecnum{0}% \def\thissubsecnum{0}% }% \def\numsecentry##1##2##3##4{% \advancenumber{chap\thischapnum}% \def\thissecnum{##2}% \def\thissubsecnum{0}% }% \def\numsubsecentry##1##2##3##4{% \advancenumber{sec\thissecnum}% \def\thissubsecnum{##2}% }% \def\numsubsubsecentry##1##2##3##4{% \advancenumber{subsec\thissubsecnum}% }% \def\thischapnum{0}% \def\thissecnum{0}% \def\thissubsecnum{0}% % % use \def rather than \let here because we redefine \chapentry et % al. a second time, below. \def\appentry{\numchapentry}% \def\appsecentry{\numsecentry}% \def\appsubsecentry{\numsubsecentry}% \def\appsubsubsecentry{\numsubsubsecentry}% \def\unnchapentry{\numchapentry}% \def\unnsecentry{\numsecentry}% \def\unnsubsecentry{\numsubsecentry}% \def\unnsubsubsecentry{\numsubsubsecentry}% \readdatafile{toc}% % % Read toc second time, this time actually producing the outlines. % The `-' means take the \expnumber as the absolute number of % subentries, which we calculated on our first read of the .toc above. % % We use the node names as the destinations. \def\numchapentry##1##2##3##4{% \dopdfoutline{##1}{count-\expnumber{chap##2}}{##3}{##4}}% \def\numsecentry##1##2##3##4{% \dopdfoutline{##1}{count-\expnumber{sec##2}}{##3}{##4}}% \def\numsubsecentry##1##2##3##4{% \dopdfoutline{##1}{count-\expnumber{subsec##2}}{##3}{##4}}% \def\numsubsubsecentry##1##2##3##4{% count is always zero \dopdfoutline{##1}{}{##3}{##4}}% % % PDF outlines are displayed using system fonts, instead of % document fonts. Therefore we cannot use special characters, % since the encoding is unknown. For example, the eogonek from % Latin 2 (0xea) gets translated to a | character. Info from % Staszek Wawrykiewicz, 19 Jan 2004 04:09:24 +0100. % % TODO this right, we have to translate 8-bit characters to % their "best" equivalent, based on the @documentencoding. Too % much work for too little return. Just use the ASCII equivalents % we use for the index sort strings. % \indexnofonts \setupdatafile % We can have normal brace characters in the PDF outlines, unlike % Texinfo index files. So set that up. \def\{{\lbracecharliteral}% \def\}{\rbracecharliteral}% \catcode`\\=\active \otherbackslash \input \tocreadfilename \endgroup } {\catcode`[=1 \catcode`]=2 \catcode`{=\other \catcode`}=\other \gdef\lbracecharliteral[{]% \gdef\rbracecharliteral[}]% ] % \def\skipspaces#1{\def\PP{#1}\def\D{|}% \ifx\PP\D\let\nextsp\relax \else\let\nextsp\skipspaces \addtokens{\filename}{\PP}% \advance\filenamelength by 1 \fi \nextsp} \def\getfilename#1{% \filenamelength=0 % If we don't expand the argument now, \skipspaces will get % snagged on things like "@value{foo}". \edef\temp{#1}% \expandafter\skipspaces\temp|\relax } \ifnum\pdftexversion < 14 \let \startlink \pdfannotlink \else \let \startlink \pdfstartlink \fi % make a live url in pdf output. \def\pdfurl#1{% \begingroup % it seems we really need yet another set of dummies; have not % tried to figure out what each command should do in the context % of @url. for now, just make @/ a no-op, that's the only one % people have actually reported a problem with. % \normalturnoffactive \def\@{@}% \let\/=\empty \makevalueexpandable % do we want to go so far as to use \indexnofonts instead of just % special-casing \var here? \def\var##1{##1}% % \leavevmode\setcolor{\urlcolor}% \startlink attr{/Border [0 0 0]}% user{/Subtype /Link /A << /S /URI /URI (#1) >>}% \endgroup} \def\pdfgettoks#1.{\setbox\boxA=\hbox{\toksA={#1.}\toksB={}\maketoks}} \def\addtokens#1#2{\edef\addtoks{\noexpand#1={\the#1#2}}\addtoks} \def\adn#1{\addtokens{\toksC}{#1}\global\countA=1\let\next=\maketoks} \def\poptoks#1#2|ENDTOKS|{\let\first=#1\toksD={#1}\toksA={#2}} \def\maketoks{% \expandafter\poptoks\the\toksA|ENDTOKS|\relax \ifx\first0\adn0 \else\ifx\first1\adn1 \else\ifx\first2\adn2 \else\ifx\first3\adn3 \else\ifx\first4\adn4 \else\ifx\first5\adn5 \else\ifx\first6\adn6 \else\ifx\first7\adn7 \else\ifx\first8\adn8 \else\ifx\first9\adn9 \else \ifnum0=\countA\else\makelink\fi \ifx\first.\let\next=\done\else \let\next=\maketoks \addtokens{\toksB}{\the\toksD} \ifx\first,\addtokens{\toksB}{\space}\fi \fi \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi \next} \def\makelink{\addtokens{\toksB}% {\noexpand\pdflink{\the\toksC}}\toksC={}\global\countA=0} \def\pdflink#1{% \startlink attr{/Border [0 0 0]} goto name{\pdfmkpgn{#1}} \setcolor{\linkcolor}#1\endlink} \def\done{\edef\st{\global\noexpand\toksA={\the\toksB}}\st} \else % non-pdf mode \let\pdfmkdest = \gobble \let\pdfurl = \gobble \let\endlink = \relax \let\setcolor = \gobble \let\pdfsetcolor = \gobble \let\pdfmakeoutlines = \relax \fi % \ifx\pdfoutput % % For XeTeX % \ifx\XeTeXrevision\thisisundefined \else % % XeTeX version check % \ifnum\strcmp{\the\XeTeXversion\XeTeXrevision}{0.99996}>-1 % TeX Live 2016 contains XeTeX 0.99996 and xdvipdfmx 20160307. % It can use the `dvipdfmx:config' special (from TeX Live SVN r40941). % For avoiding PDF destination name replacement, we use this special % instead of xdvipdfmx's command line option `-C 0x0010'. \special{dvipdfmx:config C 0x0010} % XeTeX 0.99995+ comes with xdvipdfmx 20160307+. % It can handle Unicode destination names for PDF. \txiuseunicodedestnametrue \else % XeTeX < 0.99996 (TeX Live < 2016) cannot use the % `dvipdfmx:config' special. % So for avoiding PDF destination name replacement, % xdvipdfmx's command line option `-C 0x0010' is necessary. % % XeTeX < 0.99995 can not handle Unicode destination names for PDF % because xdvipdfmx 20150315 has a UTF-16 conversion issue. % It is fixed by xdvipdfmx 20160106 (TeX Live SVN r39753). \txiuseunicodedestnamefalse \fi % % Color support % \def\rgbDarkRed{0.50 0.09 0.12} \def\rgbBlack{0 0 0} % \def\pdfsetcolor#1{\special{pdf:scolor [#1]}} % % Set color, and create a mark which defines \thiscolor accordingly, % so that \makeheadline knows which color to restore. \def\setcolor#1{% \xdef\lastcolordefs{\gdef\noexpand\thiscolor{#1}}% \domark \pdfsetcolor{#1}% } % \def\maincolor{\rgbBlack} \pdfsetcolor{\maincolor} \edef\thiscolor{\maincolor} \def\lastcolordefs{} % \def\makefootline{% \baselineskip24pt \line{\pdfsetcolor{\maincolor}\the\footline}% } % \def\makeheadline{% \vbox to 0pt{% \vskip-22.5pt \line{% \vbox to8.5pt{}% % Extract \thiscolor definition from the marks. \getcolormarks % Typeset the headline with \maincolor, then restore the color. \pdfsetcolor{\maincolor}\the\headline\pdfsetcolor{\thiscolor}% }% \vss }% \nointerlineskip } % % PDF outline support % % Emulate pdfTeX primitive \def\pdfdest name#1 xyz{% \special{pdf:dest (#1) [@thispage /XYZ @xpos @ypos null]}% } % \def\setpdfdestname#1{{% % We have to set dummies so commands such as @code, and characters % such as \, aren't expanded when present in a section title. \indexnofonts \makevalueexpandable \turnoffactive \iftxiuseunicodedestname % Pass through Unicode characters. \else % Use ASCII approximations in destination names. \passthroughcharsfalse \fi \def\pdfdestname{#1}% \txiescapepdf\pdfdestname }} % \def\setpdfoutlinetext#1{{% \turnoffactive % Always use Unicode characters in title texts. \def\pdfoutlinetext{#1}% % For XeTeX, xdvipdfmx converts to UTF-16. % So we do not convert. \txiescapepdf\pdfoutlinetext }} % \def\pdfmkdest#1{% \setpdfdestname{#1}% \safewhatsit{\pdfdest name{\pdfdestname} xyz}% } % % by default, use black for everything. \def\urlcolor{\rgbBlack} \def\linkcolor{\rgbBlack} \def\endlink{\setcolor{\maincolor}\pdfendlink} % \def\dopdfoutline#1#2#3#4{% \setpdfoutlinetext{#1} \setpdfdestname{#3} \ifx\pdfdestname\empty \def\pdfdestname{#4}% \fi % \special{pdf:out [-] #2 << /Title (\pdfoutlinetext) /A << /S /GoTo /D (\pdfdestname) >> >> }% } % \def\pdfmakeoutlines{% \begingroup % % For XeTeX, counts of subentries are not necessary. % Therefore, we read toc only once. % % We use node names as destinations. \def\partentry##1##2##3##4{}% ignore parts in the outlines \def\numchapentry##1##2##3##4{% \dopdfoutline{##1}{1}{##3}{##4}}% \def\numsecentry##1##2##3##4{% \dopdfoutline{##1}{2}{##3}{##4}}% \def\numsubsecentry##1##2##3##4{% \dopdfoutline{##1}{3}{##3}{##4}}% \def\numsubsubsecentry##1##2##3##4{% \dopdfoutline{##1}{4}{##3}{##4}}% % \let\appentry\numchapentry% \let\appsecentry\numsecentry% \let\appsubsecentry\numsubsecentry% \let\appsubsubsecentry\numsubsubsecentry% \let\unnchapentry\numchapentry% \let\unnsecentry\numsecentry% \let\unnsubsecentry\numsubsecentry% \let\unnsubsubsecentry\numsubsubsecentry% % % For XeTeX, xdvipdfmx converts strings to UTF-16. % Therefore, the encoding and the language may not be considered. % \indexnofonts \setupdatafile % We can have normal brace characters in the PDF outlines, unlike % Texinfo index files. So set that up. \def\{{\lbracecharliteral}% \def\}{\rbracecharliteral}% \catcode`\\=\active \otherbackslash \input \tocreadfilename \endgroup } {\catcode`[=1 \catcode`]=2 \catcode`{=\other \catcode`}=\other \gdef\lbracecharliteral[{]% \gdef\rbracecharliteral[}]% ] \special{pdf:docview << /PageMode /UseOutlines >> } % ``\special{pdf:tounicode ...}'' is not necessary % because xdvipdfmx converts strings from UTF-8 to UTF-16 without it. % However, due to a UTF-16 conversion issue of xdvipdfmx 20150315, % ``\special{pdf:dest ...}'' cannot handle non-ASCII strings. % It is fixed by xdvipdfmx 20160106 (TeX Live SVN r39753). % \def\skipspaces#1{\def\PP{#1}\def\D{|}% \ifx\PP\D\let\nextsp\relax \else\let\nextsp\skipspaces \addtokens{\filename}{\PP}% \advance\filenamelength by 1 \fi \nextsp} \def\getfilename#1{% \filenamelength=0 % If we don't expand the argument now, \skipspaces will get % snagged on things like "@value{foo}". \edef\temp{#1}% \expandafter\skipspaces\temp|\relax } % make a live url in pdf output. \def\pdfurl#1{% \begingroup % it seems we really need yet another set of dummies; have not % tried to figure out what each command should do in the context % of @url. for now, just make @/ a no-op, that's the only one % people have actually reported a problem with. % \normalturnoffactive \def\@{@}% \let\/=\empty \makevalueexpandable % do we want to go so far as to use \indexnofonts instead of just % special-casing \var here? \def\var##1{##1}% % \leavevmode\setcolor{\urlcolor}% \special{pdf:bann << /Border [0 0 0] /Subtype /Link /A << /S /URI /URI (#1) >> >>}% \endgroup} \def\endlink{\setcolor{\maincolor}\special{pdf:eann}} \def\pdfgettoks#1.{\setbox\boxA=\hbox{\toksA={#1.}\toksB={}\maketoks}} \def\addtokens#1#2{\edef\addtoks{\noexpand#1={\the#1#2}}\addtoks} \def\adn#1{\addtokens{\toksC}{#1}\global\countA=1\let\next=\maketoks} \def\poptoks#1#2|ENDTOKS|{\let\first=#1\toksD={#1}\toksA={#2}} \def\maketoks{% \expandafter\poptoks\the\toksA|ENDTOKS|\relax \ifx\first0\adn0 \else\ifx\first1\adn1 \else\ifx\first2\adn2 \else\ifx\first3\adn3 \else\ifx\first4\adn4 \else\ifx\first5\adn5 \else\ifx\first6\adn6 \else\ifx\first7\adn7 \else\ifx\first8\adn8 \else\ifx\first9\adn9 \else \ifnum0=\countA\else\makelink\fi \ifx\first.\let\next=\done\else \let\next=\maketoks \addtokens{\toksB}{\the\toksD} \ifx\first,\addtokens{\toksB}{\space}\fi \fi \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi \next} \def\makelink{\addtokens{\toksB}% {\noexpand\pdflink{\the\toksC}}\toksC={}\global\countA=0} \def\pdflink#1{% \special{pdf:bann << /Border [0 0 0] /Type /Annot /Subtype /Link /A << /S /GoTo /D (#1) >> >>}% \setcolor{\linkcolor}#1\endlink} \def\done{\edef\st{\global\noexpand\toksA={\the\toksB}}\st} % % % @image support % % #1 is image name, #2 width (might be empty/whitespace), #3 height (ditto). \def\doxeteximage#1#2#3{% \def\xeteximagewidth{#2}\setbox0 = \hbox{\ignorespaces #2}% \def\xeteximageheight{#3}\setbox2 = \hbox{\ignorespaces #3}% % % XeTeX (and the PDF format) supports .pdf, .png, .jpg (among % others). Let's try in that order, PDF first since if % someone has a scalable image, presumably better to use that than a % bitmap. \let\xeteximgext=\empty \begingroup \openin 1 #1.pdf \ifeof 1 \openin 1 #1.PDF \ifeof 1 \openin 1 #1.png \ifeof 1 \openin 1 #1.jpg \ifeof 1 \openin 1 #1.jpeg \ifeof 1 \openin 1 #1.JPG \ifeof 1 \errmessage{Could not find image file #1 for XeTeX}% \else \gdef\xeteximgext{JPG}% \fi \else \gdef\xeteximgext{jpeg}% \fi \else \gdef\xeteximgext{jpg}% \fi \else \gdef\xeteximgext{png}% \fi \else \gdef\xeteximgext{PDF}% \fi \else \gdef\xeteximgext{pdf}% \fi \closein 1 \endgroup % \def\xetexpdfext{pdf}% \ifx\xeteximgext\xetexpdfext \XeTeXpdffile "#1".\xeteximgext "" \else \def\xetexpdfext{PDF}% \ifx\xeteximgext\xetexpdfext \XeTeXpdffile "#1".\xeteximgext "" \else \XeTeXpicfile "#1".\xeteximgext "" \fi \fi \ifdim \wd0 >0pt width \xeteximagewidth \fi \ifdim \wd2 >0pt height \xeteximageheight \fi \relax } \fi % \message{fonts,} % Set the baselineskip to #1, and the lineskip and strut size % correspondingly. There is no deep meaning behind these magic numbers % used as factors; they just match (closely enough) what Knuth defined. % \def\lineskipfactor{.08333} \def\strutheightpercent{.70833} \def\strutdepthpercent {.29167} % % can get a sort of poor man's double spacing by redefining this. \def\baselinefactor{1} % \newdimen\textleading \def\setleading#1{% \dimen0 = #1\relax \normalbaselineskip = \baselinefactor\dimen0 \normallineskip = \lineskipfactor\normalbaselineskip \normalbaselines \setbox\strutbox =\hbox{% \vrule width0pt height\strutheightpercent\baselineskip depth \strutdepthpercent \baselineskip }% } % PDF CMaps. See also LaTeX's t1.cmap. % % do nothing with this by default. \expandafter\let\csname cmapOT1\endcsname\gobble \expandafter\let\csname cmapOT1IT\endcsname\gobble \expandafter\let\csname cmapOT1TT\endcsname\gobble % if we are producing pdf, and we have \pdffontattr, then define cmaps. % (\pdffontattr was introduced many years ago, but people still run % older pdftex's; it's easy to conditionalize, so we do.) \ifpdf \ifx\pdffontattr\thisisundefined \else \begingroup \catcode`\^^M=\active \def^^M{^^J}% Output line endings as the ^^J char. \catcode`\%=12 \immediate\pdfobj stream {%!PS-Adobe-3.0 Resource-CMap %%DocumentNeededResources: ProcSet (CIDInit) %%IncludeResource: ProcSet (CIDInit) %%BeginResource: CMap (TeX-OT1-0) %%Title: (TeX-OT1-0 TeX OT1 0) %%Version: 1.000 %%EndComments /CIDInit /ProcSet findresource begin 12 dict begin begincmap /CIDSystemInfo << /Registry (TeX) /Ordering (OT1) /Supplement 0 >> def /CMapName /TeX-OT1-0 def /CMapType 2 def 1 begincodespacerange <00> <7F> endcodespacerange 8 beginbfrange <00> <01> <0393> <09> <0A> <03A8> <23> <26> <0023> <28> <3B> <0028> <3F> <5B> <003F> <5D> <5E> <005D> <61> <7A> <0061> <7B> <7C> <2013> endbfrange 40 beginbfchar <02> <0398> <03> <039B> <04> <039E> <05> <03A0> <06> <03A3> <07> <03D2> <08> <03A6> <0B> <00660066> <0C> <00660069> <0D> <0066006C> <0E> <006600660069> <0F> <00660066006C> <10> <0131> <11> <0237> <12> <0060> <13> <00B4> <14> <02C7> <15> <02D8> <16> <00AF> <17> <02DA> <18> <00B8> <19> <00DF> <1A> <00E6> <1B> <0153> <1C> <00F8> <1D> <00C6> <1E> <0152> <1F> <00D8> <21> <0021> <22> <201D> <27> <2019> <3C> <00A1> <3D> <003D> <3E> <00BF> <5C> <201C> <5F> <02D9> <60> <2018> <7D> <02DD> <7E> <007E> <7F> <00A8> endbfchar endcmap CMapName currentdict /CMap defineresource pop end end %%EndResource %%EOF }\endgroup \expandafter\edef\csname cmapOT1\endcsname#1{% \pdffontattr#1{/ToUnicode \the\pdflastobj\space 0 R}% }% % % \cmapOT1IT \begingroup \catcode`\^^M=\active \def^^M{^^J}% Output line endings as the ^^J char. \catcode`\%=12 \immediate\pdfobj stream {%!PS-Adobe-3.0 Resource-CMap %%DocumentNeededResources: ProcSet (CIDInit) %%IncludeResource: ProcSet (CIDInit) %%BeginResource: CMap (TeX-OT1IT-0) %%Title: (TeX-OT1IT-0 TeX OT1IT 0) %%Version: 1.000 %%EndComments /CIDInit /ProcSet findresource begin 12 dict begin begincmap /CIDSystemInfo << /Registry (TeX) /Ordering (OT1IT) /Supplement 0 >> def /CMapName /TeX-OT1IT-0 def /CMapType 2 def 1 begincodespacerange <00> <7F> endcodespacerange 8 beginbfrange <00> <01> <0393> <09> <0A> <03A8> <25> <26> <0025> <28> <3B> <0028> <3F> <5B> <003F> <5D> <5E> <005D> <61> <7A> <0061> <7B> <7C> <2013> endbfrange 42 beginbfchar <02> <0398> <03> <039B> <04> <039E> <05> <03A0> <06> <03A3> <07> <03D2> <08> <03A6> <0B> <00660066> <0C> <00660069> <0D> <0066006C> <0E> <006600660069> <0F> <00660066006C> <10> <0131> <11> <0237> <12> <0060> <13> <00B4> <14> <02C7> <15> <02D8> <16> <00AF> <17> <02DA> <18> <00B8> <19> <00DF> <1A> <00E6> <1B> <0153> <1C> <00F8> <1D> <00C6> <1E> <0152> <1F> <00D8> <21> <0021> <22> <201D> <23> <0023> <24> <00A3> <27> <2019> <3C> <00A1> <3D> <003D> <3E> <00BF> <5C> <201C> <5F> <02D9> <60> <2018> <7D> <02DD> <7E> <007E> <7F> <00A8> endbfchar endcmap CMapName currentdict /CMap defineresource pop end end %%EndResource %%EOF }\endgroup \expandafter\edef\csname cmapOT1IT\endcsname#1{% \pdffontattr#1{/ToUnicode \the\pdflastobj\space 0 R}% }% % % \cmapOT1TT \begingroup \catcode`\^^M=\active \def^^M{^^J}% Output line endings as the ^^J char. \catcode`\%=12 \immediate\pdfobj stream {%!PS-Adobe-3.0 Resource-CMap %%DocumentNeededResources: ProcSet (CIDInit) %%IncludeResource: ProcSet (CIDInit) %%BeginResource: CMap (TeX-OT1TT-0) %%Title: (TeX-OT1TT-0 TeX OT1TT 0) %%Version: 1.000 %%EndComments /CIDInit /ProcSet findresource begin 12 dict begin begincmap /CIDSystemInfo << /Registry (TeX) /Ordering (OT1TT) /Supplement 0 >> def /CMapName /TeX-OT1TT-0 def /CMapType 2 def 1 begincodespacerange <00> <7F> endcodespacerange 5 beginbfrange <00> <01> <0393> <09> <0A> <03A8> <21> <26> <0021> <28> <5F> <0028> <61> <7E> <0061> endbfrange 32 beginbfchar <02> <0398> <03> <039B> <04> <039E> <05> <03A0> <06> <03A3> <07> <03D2> <08> <03A6> <0B> <2191> <0C> <2193> <0D> <0027> <0E> <00A1> <0F> <00BF> <10> <0131> <11> <0237> <12> <0060> <13> <00B4> <14> <02C7> <15> <02D8> <16> <00AF> <17> <02DA> <18> <00B8> <19> <00DF> <1A> <00E6> <1B> <0153> <1C> <00F8> <1D> <00C6> <1E> <0152> <1F> <00D8> <20> <2423> <27> <2019> <60> <2018> <7F> <00A8> endbfchar endcmap CMapName currentdict /CMap defineresource pop end end %%EndResource %%EOF }\endgroup \expandafter\edef\csname cmapOT1TT\endcsname#1{% \pdffontattr#1{/ToUnicode \the\pdflastobj\space 0 R}% }% \fi\fi % Set the font macro #1 to the font named \fontprefix#2. % #3 is the font's design size, #4 is a scale factor, #5 is the CMap % encoding (only OT1, OT1IT and OT1TT are allowed, or empty to omit). % Example: % #1 = \textrm % #2 = \rmshape % #3 = 10 % #4 = \mainmagstep % #5 = OT1 % \def\setfont#1#2#3#4#5{% \font#1=\fontprefix#2#3 scaled #4 \csname cmap#5\endcsname#1% } % This is what gets called when #5 of \setfont is empty. \let\cmap\gobble % % (end of cmaps) % Use cm as the default font prefix. % To specify the font prefix, you must define \fontprefix % before you read in texinfo.tex. \ifx\fontprefix\thisisundefined \def\fontprefix{cm} \fi % Support font families that don't use the same naming scheme as CM. \def\rmshape{r} \def\rmbshape{bx} % where the normal face is bold \def\bfshape{b} \def\bxshape{bx} \def\ttshape{tt} \def\ttbshape{tt} \def\ttslshape{sltt} \def\itshape{ti} \def\itbshape{bxti} \def\slshape{sl} \def\slbshape{bxsl} \def\sfshape{ss} \def\sfbshape{ss} \def\scshape{csc} \def\scbshape{csc} % Definitions for a main text size of 11pt. (The default in Texinfo.) % \def\definetextfontsizexi{% % Text fonts (11.2pt, magstep1). \def\textnominalsize{11pt} \edef\mainmagstep{\magstephalf} \setfont\textrm\rmshape{10}{\mainmagstep}{OT1} \setfont\texttt\ttshape{10}{\mainmagstep}{OT1TT} \setfont\textbf\bfshape{10}{\mainmagstep}{OT1} \setfont\textit\itshape{10}{\mainmagstep}{OT1IT} \setfont\textsl\slshape{10}{\mainmagstep}{OT1} \setfont\textsf\sfshape{10}{\mainmagstep}{OT1} \setfont\textsc\scshape{10}{\mainmagstep}{OT1} \setfont\textttsl\ttslshape{10}{\mainmagstep}{OT1TT} \font\texti=cmmi10 scaled \mainmagstep \font\textsy=cmsy10 scaled \mainmagstep \def\textecsize{1095} % A few fonts for @defun names and args. \setfont\defbf\bfshape{10}{\magstep1}{OT1} \setfont\deftt\ttshape{10}{\magstep1}{OT1TT} \setfont\defsl\slshape{10}{\magstep1}{OT1TT} \setfont\defttsl\ttslshape{10}{\magstep1}{OT1TT} \def\df{\let\ttfont=\deftt \let\bffont = \defbf \let\ttslfont=\defttsl \let\slfont=\defsl \bf} % Fonts for indices, footnotes, small examples (9pt). \def\smallnominalsize{9pt} \setfont\smallrm\rmshape{9}{1000}{OT1} \setfont\smalltt\ttshape{9}{1000}{OT1TT} \setfont\smallbf\bfshape{10}{900}{OT1} \setfont\smallit\itshape{9}{1000}{OT1IT} \setfont\smallsl\slshape{9}{1000}{OT1} \setfont\smallsf\sfshape{9}{1000}{OT1} \setfont\smallsc\scshape{10}{900}{OT1} \setfont\smallttsl\ttslshape{10}{900}{OT1TT} \font\smalli=cmmi9 \font\smallsy=cmsy9 \def\smallecsize{0900} % Fonts for small examples (8pt). \def\smallernominalsize{8pt} \setfont\smallerrm\rmshape{8}{1000}{OT1} \setfont\smallertt\ttshape{8}{1000}{OT1TT} \setfont\smallerbf\bfshape{10}{800}{OT1} \setfont\smallerit\itshape{8}{1000}{OT1IT} \setfont\smallersl\slshape{8}{1000}{OT1} \setfont\smallersf\sfshape{8}{1000}{OT1} \setfont\smallersc\scshape{10}{800}{OT1} \setfont\smallerttsl\ttslshape{10}{800}{OT1TT} \font\smalleri=cmmi8 \font\smallersy=cmsy8 \def\smallerecsize{0800} % Fonts for title page (20.4pt): \def\titlenominalsize{20pt} \setfont\titlerm\rmbshape{12}{\magstep3}{OT1} \setfont\titleit\itbshape{10}{\magstep4}{OT1IT} \setfont\titlesl\slbshape{10}{\magstep4}{OT1} \setfont\titlett\ttbshape{12}{\magstep3}{OT1TT} \setfont\titlettsl\ttslshape{10}{\magstep4}{OT1TT} \setfont\titlesf\sfbshape{17}{\magstep1}{OT1} \let\titlebf=\titlerm \setfont\titlesc\scbshape{10}{\magstep4}{OT1} \font\titlei=cmmi12 scaled \magstep3 \font\titlesy=cmsy10 scaled \magstep4 \def\titleecsize{2074} % Chapter (and unnumbered) fonts (17.28pt). \def\chapnominalsize{17pt} \setfont\chaprm\rmbshape{12}{\magstep2}{OT1} \setfont\chapit\itbshape{10}{\magstep3}{OT1IT} \setfont\chapsl\slbshape{10}{\magstep3}{OT1} \setfont\chaptt\ttbshape{12}{\magstep2}{OT1TT} \setfont\chapttsl\ttslshape{10}{\magstep3}{OT1TT} \setfont\chapsf\sfbshape{17}{1000}{OT1} \let\chapbf=\chaprm \setfont\chapsc\scbshape{10}{\magstep3}{OT1} \font\chapi=cmmi12 scaled \magstep2 \font\chapsy=cmsy10 scaled \magstep3 \def\chapecsize{1728} % Section fonts (14.4pt). \def\secnominalsize{14pt} \setfont\secrm\rmbshape{12}{\magstep1}{OT1} \setfont\secrmnotbold\rmshape{12}{\magstep1}{OT1} \setfont\secit\itbshape{10}{\magstep2}{OT1IT} \setfont\secsl\slbshape{10}{\magstep2}{OT1} \setfont\sectt\ttbshape{12}{\magstep1}{OT1TT} \setfont\secttsl\ttslshape{10}{\magstep2}{OT1TT} \setfont\secsf\sfbshape{12}{\magstep1}{OT1} \let\secbf\secrm \setfont\secsc\scbshape{10}{\magstep2}{OT1} \font\seci=cmmi12 scaled \magstep1 \font\secsy=cmsy10 scaled \magstep2 \def\sececsize{1440} % Subsection fonts (13.15pt). \def\ssecnominalsize{13pt} \setfont\ssecrm\rmbshape{12}{\magstephalf}{OT1} \setfont\ssecit\itbshape{10}{1315}{OT1IT} \setfont\ssecsl\slbshape{10}{1315}{OT1} \setfont\ssectt\ttbshape{12}{\magstephalf}{OT1TT} \setfont\ssecttsl\ttslshape{10}{1315}{OT1TT} \setfont\ssecsf\sfbshape{12}{\magstephalf}{OT1} \let\ssecbf\ssecrm \setfont\ssecsc\scbshape{10}{1315}{OT1} \font\sseci=cmmi12 scaled \magstephalf \font\ssecsy=cmsy10 scaled 1315 \def\ssececsize{1200} % Reduced fonts for @acronym in text (10pt). \def\reducednominalsize{10pt} \setfont\reducedrm\rmshape{10}{1000}{OT1} \setfont\reducedtt\ttshape{10}{1000}{OT1TT} \setfont\reducedbf\bfshape{10}{1000}{OT1} \setfont\reducedit\itshape{10}{1000}{OT1IT} \setfont\reducedsl\slshape{10}{1000}{OT1} \setfont\reducedsf\sfshape{10}{1000}{OT1} \setfont\reducedsc\scshape{10}{1000}{OT1} \setfont\reducedttsl\ttslshape{10}{1000}{OT1TT} \font\reducedi=cmmi10 \font\reducedsy=cmsy10 \def\reducedecsize{1000} \textleading = 13.2pt % line spacing for 11pt CM \textfonts % reset the current fonts \rm } % end of 11pt text font size definitions, \definetextfontsizexi % Definitions to make the main text be 10pt Computer Modern, with % section, chapter, etc., sizes following suit. This is for the GNU % Press printing of the Emacs 22 manual. Maybe other manuals in the % future. Used with @smallbook, which sets the leading to 12pt. % \def\definetextfontsizex{% % Text fonts (10pt). \def\textnominalsize{10pt} \edef\mainmagstep{1000} \setfont\textrm\rmshape{10}{\mainmagstep}{OT1} \setfont\texttt\ttshape{10}{\mainmagstep}{OT1TT} \setfont\textbf\bfshape{10}{\mainmagstep}{OT1} \setfont\textit\itshape{10}{\mainmagstep}{OT1IT} \setfont\textsl\slshape{10}{\mainmagstep}{OT1} \setfont\textsf\sfshape{10}{\mainmagstep}{OT1} \setfont\textsc\scshape{10}{\mainmagstep}{OT1} \setfont\textttsl\ttslshape{10}{\mainmagstep}{OT1TT} \font\texti=cmmi10 scaled \mainmagstep \font\textsy=cmsy10 scaled \mainmagstep \def\textecsize{1000} % A few fonts for @defun names and args. \setfont\defbf\bfshape{10}{\magstephalf}{OT1} \setfont\deftt\ttshape{10}{\magstephalf}{OT1TT} \setfont\defsl\slshape{10}{\magstephalf}{OT1TT} \setfont\defttsl\ttslshape{10}{\magstephalf}{OT1TT} \def\df{\let\ttfont=\deftt \let\bffont = \defbf \let\slfont=\defsl \let\ttslfont=\defttsl \bf} % Fonts for indices, footnotes, small examples (9pt). \def\smallnominalsize{9pt} \setfont\smallrm\rmshape{9}{1000}{OT1} \setfont\smalltt\ttshape{9}{1000}{OT1TT} \setfont\smallbf\bfshape{10}{900}{OT1} \setfont\smallit\itshape{9}{1000}{OT1IT} \setfont\smallsl\slshape{9}{1000}{OT1} \setfont\smallsf\sfshape{9}{1000}{OT1} \setfont\smallsc\scshape{10}{900}{OT1} \setfont\smallttsl\ttslshape{10}{900}{OT1TT} \font\smalli=cmmi9 \font\smallsy=cmsy9 \def\smallecsize{0900} % Fonts for small examples (8pt). \def\smallernominalsize{8pt} \setfont\smallerrm\rmshape{8}{1000}{OT1} \setfont\smallertt\ttshape{8}{1000}{OT1TT} \setfont\smallerbf\bfshape{10}{800}{OT1} \setfont\smallerit\itshape{8}{1000}{OT1IT} \setfont\smallersl\slshape{8}{1000}{OT1} \setfont\smallersf\sfshape{8}{1000}{OT1} \setfont\smallersc\scshape{10}{800}{OT1} \setfont\smallerttsl\ttslshape{10}{800}{OT1TT} \font\smalleri=cmmi8 \font\smallersy=cmsy8 \def\smallerecsize{0800} % Fonts for title page (20.4pt): \def\titlenominalsize{20pt} \setfont\titlerm\rmbshape{12}{\magstep3}{OT1} \setfont\titleit\itbshape{10}{\magstep4}{OT1IT} \setfont\titlesl\slbshape{10}{\magstep4}{OT1} \setfont\titlett\ttbshape{12}{\magstep3}{OT1TT} \setfont\titlettsl\ttslshape{10}{\magstep4}{OT1TT} \setfont\titlesf\sfbshape{17}{\magstep1}{OT1} \let\titlebf=\titlerm \setfont\titlesc\scbshape{10}{\magstep4}{OT1} \font\titlei=cmmi12 scaled \magstep3 \font\titlesy=cmsy10 scaled \magstep4 \def\titleecsize{2074} % Chapter fonts (14.4pt). \def\chapnominalsize{14pt} \setfont\chaprm\rmbshape{12}{\magstep1}{OT1} \setfont\chapit\itbshape{10}{\magstep2}{OT1IT} \setfont\chapsl\slbshape{10}{\magstep2}{OT1} \setfont\chaptt\ttbshape{12}{\magstep1}{OT1TT} \setfont\chapttsl\ttslshape{10}{\magstep2}{OT1TT} \setfont\chapsf\sfbshape{12}{\magstep1}{OT1} \let\chapbf\chaprm \setfont\chapsc\scbshape{10}{\magstep2}{OT1} \font\chapi=cmmi12 scaled \magstep1 \font\chapsy=cmsy10 scaled \magstep2 \def\chapecsize{1440} % Section fonts (12pt). \def\secnominalsize{12pt} \setfont\secrm\rmbshape{12}{1000}{OT1} \setfont\secit\itbshape{10}{\magstep1}{OT1IT} \setfont\secsl\slbshape{10}{\magstep1}{OT1} \setfont\sectt\ttbshape{12}{1000}{OT1TT} \setfont\secttsl\ttslshape{10}{\magstep1}{OT1TT} \setfont\secsf\sfbshape{12}{1000}{OT1} \let\secbf\secrm \setfont\secsc\scbshape{10}{\magstep1}{OT1} \font\seci=cmmi12 \font\secsy=cmsy10 scaled \magstep1 \def\sececsize{1200} % Subsection fonts (10pt). \def\ssecnominalsize{10pt} \setfont\ssecrm\rmbshape{10}{1000}{OT1} \setfont\ssecit\itbshape{10}{1000}{OT1IT} \setfont\ssecsl\slbshape{10}{1000}{OT1} \setfont\ssectt\ttbshape{10}{1000}{OT1TT} \setfont\ssecttsl\ttslshape{10}{1000}{OT1TT} \setfont\ssecsf\sfbshape{10}{1000}{OT1} \let\ssecbf\ssecrm \setfont\ssecsc\scbshape{10}{1000}{OT1} \font\sseci=cmmi10 \font\ssecsy=cmsy10 \def\ssececsize{1000} % Reduced fonts for @acronym in text (9pt). \def\reducednominalsize{9pt} \setfont\reducedrm\rmshape{9}{1000}{OT1} \setfont\reducedtt\ttshape{9}{1000}{OT1TT} \setfont\reducedbf\bfshape{10}{900}{OT1} \setfont\reducedit\itshape{9}{1000}{OT1IT} \setfont\reducedsl\slshape{9}{1000}{OT1} \setfont\reducedsf\sfshape{9}{1000}{OT1} \setfont\reducedsc\scshape{10}{900}{OT1} \setfont\reducedttsl\ttslshape{10}{900}{OT1TT} \font\reducedi=cmmi9 \font\reducedsy=cmsy9 \def\reducedecsize{0900} \divide\parskip by 2 % reduce space between paragraphs \textleading = 12pt % line spacing for 10pt CM \textfonts % reset the current fonts \rm } % end of 10pt text font size definitions, \definetextfontsizex % Fonts for short table of contents. \setfont\shortcontrm\rmshape{12}{1000}{OT1} \setfont\shortcontbf\bfshape{10}{\magstep1}{OT1} % no cmb12 \setfont\shortcontsl\slshape{12}{1000}{OT1} \setfont\shortconttt\ttshape{12}{1000}{OT1TT} % We provide the user-level command % @fonttextsize 10 % (or 11) to redefine the text font size. pt is assumed. % \def\xiword{11} \def\xword{10} \def\xwordpt{10pt} % \parseargdef\fonttextsize{% \def\textsizearg{#1}% %\wlog{doing @fonttextsize \textsizearg}% % % Set \globaldefs so that documents can use this inside @tex, since % makeinfo 4.8 does not support it, but we need it nonetheless. % \begingroup \globaldefs=1 \ifx\textsizearg\xword \definetextfontsizex \else \ifx\textsizearg\xiword \definetextfontsizexi \else \errhelp=\EMsimple \errmessage{@fonttextsize only supports `10' or `11', not `\textsizearg'} \fi\fi \endgroup } % % Change the current font style to #1, remembering it in \curfontstyle. % For now, we do not accumulate font styles: @b{@i{foo}} prints foo in % italics, not bold italics. % \def\setfontstyle#1{% \def\curfontstyle{#1}% not as a control sequence, because we are \edef'd. \csname #1font\endcsname % change the current font } \def\rm{\fam=0 \setfontstyle{rm}} \def\it{\fam=\itfam \setfontstyle{it}} \def\sl{\fam=\slfam \setfontstyle{sl}} \def\bf{\fam=\bffam \setfontstyle{bf}}\def\bfstylename{bf} \def\tt{\fam=\ttfam \setfontstyle{tt}} % Texinfo sort of supports the sans serif font style, which plain TeX does not. % So we set up a \sf. \newfam\sffam \def\sf{\fam=\sffam \setfontstyle{sf}} % We don't need math for this font style. \def\ttsl{\setfontstyle{ttsl}} % In order for the font changes to affect most math symbols and letters, % we have to define the \textfont of the standard families. We don't % bother to reset \scriptfont and \scriptscriptfont; awaiting user need. % \def\resetmathfonts{% \textfont0=\rmfont \textfont1=\ifont \textfont2=\syfont \textfont\itfam=\itfont \textfont\slfam=\slfont \textfont\bffam=\bffont \textfont\ttfam=\ttfont \textfont\sffam=\sffont } % % The font-changing commands (all called \...fonts) redefine the meanings % of \STYLEfont, instead of just \STYLE. We do this because \STYLE needs % to also set the current \fam for math mode. Our \STYLE (e.g., \rm) % commands hardwire \STYLEfont to set the current font. % % Each font-changing command also sets the names \lsize (one size lower) % and \lllsize (three sizes lower). These relative commands are used % in, e.g., the LaTeX logo and acronyms. % % This all needs generalizing, badly. % \def\assignfonts#1{% \expandafter\let\expandafter\rmfont\csname #1rm\endcsname \expandafter\let\expandafter\itfont\csname #1it\endcsname \expandafter\let\expandafter\slfont\csname #1sl\endcsname \expandafter\let\expandafter\bffont\csname #1bf\endcsname \expandafter\let\expandafter\ttfont\csname #1tt\endcsname \expandafter\let\expandafter\smallcaps\csname #1sc\endcsname \expandafter\let\expandafter\sffont \csname #1sf\endcsname \expandafter\let\expandafter\ifont \csname #1i\endcsname \expandafter\let\expandafter\syfont \csname #1sy\endcsname \expandafter\let\expandafter\ttslfont\csname #1ttsl\endcsname } \newif\ifrmisbold % Select smaller font size with the current style. Used to change font size % in, e.g., the LaTeX logo and acronyms. If we are using bold fonts for % normal roman text, also use bold fonts for roman text in the smaller size. \def\switchtolllsize{% \expandafter\assignfonts\expandafter{\lllsize}% \ifrmisbold \let\rmfont\bffont \fi \csname\curfontstyle\endcsname }% \def\switchtolsize{% \expandafter\assignfonts\expandafter{\lsize}% \ifrmisbold \let\rmfont\bffont \fi \csname\curfontstyle\endcsname }% \def\definefontsetatsize#1#2#3#4#5{% \expandafter\def\csname #1fonts\endcsname{% \def\curfontsize{#1}% \def\lsize{#2}\def\lllsize{#3}% \csname rmisbold#5\endcsname \assignfonts{#1}% \resetmathfonts \setleading{#4}% }} \definefontsetatsize{text} {reduced}{smaller}{\textleading}{false} \definefontsetatsize{title} {chap} {subsec} {27pt} {true} \definefontsetatsize{chap} {sec} {text} {19pt} {true} \definefontsetatsize{sec} {subsec} {reduced}{17pt} {true} \definefontsetatsize{ssec} {text} {small} {15pt} {true} \definefontsetatsize{reduced}{small} {smaller}{10.5pt}{false} \definefontsetatsize{small} {smaller}{smaller}{10.5pt}{false} \definefontsetatsize{smaller}{smaller}{smaller}{9.5pt} {false} \def\titlefont#1{{\titlefonts\rm #1}} \let\subsecfonts = \ssecfonts \let\subsubsecfonts = \ssecfonts % Define these just so they can be easily changed for other fonts. \def\angleleft{$\langle$} \def\angleright{$\rangle$} % Set the fonts to use with the @small... environments. \let\smallexamplefonts = \smallfonts % About \smallexamplefonts. If we use \smallfonts (9pt), @smallexample % can fit this many characters: % 8.5x11=86 smallbook=72 a4=90 a5=69 % If we use \scriptfonts (8pt), then we can fit this many characters: % 8.5x11=90+ smallbook=80 a4=90+ a5=77 % For me, subjectively, the few extra characters that fit aren't worth % the additional smallness of 8pt. So I'm making the default 9pt. % % By the way, for comparison, here's what fits with @example (10pt): % 8.5x11=71 smallbook=60 a4=75 a5=58 % --karl, 24jan03. % Set up the default fonts, so we can use them for creating boxes. % \definetextfontsizexi \message{markup,} % Check if we are currently using a typewriter font. Since all the % Computer Modern typewriter fonts have zero interword stretch (and % shrink), and it is reasonable to expect all typewriter fonts to have % this property, we can check that font parameter. % \def\ifmonospace{\ifdim\fontdimen3\font=0pt } % Markup style infrastructure. \defmarkupstylesetup\INITMACRO will % define and register \INITMACRO to be called on markup style changes. % \INITMACRO can check \currentmarkupstyle for the innermost % style and the set of \ifmarkupSTYLE switches for all styles % currently in effect. \newif\ifmarkupvar \newif\ifmarkupsamp \newif\ifmarkupkey %\newif\ifmarkupfile % @file == @samp. %\newif\ifmarkupoption % @option == @samp. \newif\ifmarkupcode \newif\ifmarkupkbd %\newif\ifmarkupenv % @env == @code. %\newif\ifmarkupcommand % @command == @code. \newif\ifmarkuptex % @tex (and part of @math, for now). \newif\ifmarkupexample \newif\ifmarkupverb \newif\ifmarkupverbatim \let\currentmarkupstyle\empty \def\setupmarkupstyle#1{% \csname markup#1true\endcsname \def\currentmarkupstyle{#1}% \markupstylesetup } \let\markupstylesetup\empty \def\defmarkupstylesetup#1{% \expandafter\def\expandafter\markupstylesetup \expandafter{\markupstylesetup #1}% \def#1% } % Markup style setup for left and right quotes. \defmarkupstylesetup\markupsetuplq{% \expandafter\let\expandafter \temp \csname markupsetuplq\currentmarkupstyle\endcsname \ifx\temp\relax \markupsetuplqdefault \else \temp \fi } \defmarkupstylesetup\markupsetuprq{% \expandafter\let\expandafter \temp \csname markupsetuprq\currentmarkupstyle\endcsname \ifx\temp\relax \markupsetuprqdefault \else \temp \fi } { \catcode`\'=\active \catcode`\`=\active \gdef\markupsetuplqdefault{\let`\lq} \gdef\markupsetuprqdefault{\let'\rq} \gdef\markupsetcodequoteleft{\let`\codequoteleft} \gdef\markupsetcodequoteright{\let'\codequoteright} } \let\markupsetuplqcode \markupsetcodequoteleft \let\markupsetuprqcode \markupsetcodequoteright % \let\markupsetuplqexample \markupsetcodequoteleft \let\markupsetuprqexample \markupsetcodequoteright % \let\markupsetuplqkbd \markupsetcodequoteleft \let\markupsetuprqkbd \markupsetcodequoteright % \let\markupsetuplqsamp \markupsetcodequoteleft \let\markupsetuprqsamp \markupsetcodequoteright % \let\markupsetuplqverb \markupsetcodequoteleft \let\markupsetuprqverb \markupsetcodequoteright % \let\markupsetuplqverbatim \markupsetcodequoteleft \let\markupsetuprqverbatim \markupsetcodequoteright % Allow an option to not use regular directed right quote/apostrophe % (char 0x27), but instead the undirected quote from cmtt (char 0x0d). % The undirected quote is ugly, so don't make it the default, but it % works for pasting with more pdf viewers (at least evince), the % lilypond developers report. xpdf does work with the regular 0x27. % \def\codequoteright{% \expandafter\ifx\csname SETtxicodequoteundirected\endcsname\relax \expandafter\ifx\csname SETcodequoteundirected\endcsname\relax '% \else \char'15 \fi \else \char'15 \fi } % % and a similar option for the left quote char vs. a grave accent. % Modern fonts display ASCII 0x60 as a grave accent, so some people like % the code environments to do likewise. % \def\codequoteleft{% \expandafter\ifx\csname SETtxicodequotebacktick\endcsname\relax \expandafter\ifx\csname SETcodequotebacktick\endcsname\relax % [Knuth] pp. 380,381,391 % \relax disables Spanish ligatures ?` and !` of \tt font. \relax`% \else \char'22 \fi \else \char'22 \fi } % Commands to set the quote options. % \parseargdef\codequoteundirected{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETtxicodequoteundirected\endcsname = t% \else\ifx\temp\offword \expandafter\let\csname SETtxicodequoteundirected\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @codequoteundirected value `\temp', must be on|off}% \fi\fi } % \parseargdef\codequotebacktick{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETtxicodequotebacktick\endcsname = t% \else\ifx\temp\offword \expandafter\let\csname SETtxicodequotebacktick\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @codequotebacktick value `\temp', must be on|off}% \fi\fi } % [Knuth] pp. 380,381,391, disable Spanish ligatures ?` and !` of \tt font. \def\noligaturesquoteleft{\relax\lq} % Count depth in font-changes, for error checks \newcount\fontdepth \fontdepth=0 % Font commands. % #1 is the font command (\sl or \it), #2 is the text to slant. % If we are in a monospaced environment, however, 1) always use \ttsl, % and 2) do not add an italic correction. \def\dosmartslant#1#2{% \ifusingtt {{\ttsl #2}\let\next=\relax}% {\def\next{{#1#2}\futurelet\next\smartitaliccorrection}}% \next } \def\smartslanted{\dosmartslant\sl} \def\smartitalic{\dosmartslant\it} % Output an italic correction unless \next (presumed to be the following % character) is such as not to need one. \def\smartitaliccorrection{% \ifx\next,% \else\ifx\next-% \else\ifx\next.% \else\ifx\next\.% \else\ifx\next\comma% \else\ptexslash \fi\fi\fi\fi\fi \aftersmartic } % Unconditional use \ttsl, and no ic. @var is set to this for defuns. \def\ttslanted#1{{\ttsl #1}} % @cite is like \smartslanted except unconditionally use \sl. We never want % ttsl for book titles, do we? \def\cite#1{{\sl #1}\futurelet\next\smartitaliccorrection} \def\aftersmartic{} \def\var#1{% \let\saveaftersmartic = \aftersmartic \def\aftersmartic{\null\let\aftersmartic=\saveaftersmartic}% \smartslanted{#1}% } \let\i=\smartitalic \let\slanted=\smartslanted \let\dfn=\smartslanted \let\emph=\smartitalic % Explicit font changes: @r, @sc, undocumented @ii. \def\r#1{{\rm #1}} % roman font \def\sc#1{{\smallcaps#1}} % smallcaps font \def\ii#1{{\it #1}} % italic font % @b, explicit bold. Also @strong. \def\b#1{{\bf #1}} \let\strong=\b % @sansserif, explicit sans. \def\sansserif#1{{\sf #1}} % We can't just use \exhyphenpenalty, because that only has effect at % the end of a paragraph. Restore normal hyphenation at the end of the % group within which \nohyphenation is presumably called. % \def\nohyphenation{\hyphenchar\font = -1 \aftergroup\restorehyphenation} \def\restorehyphenation{\hyphenchar\font = `- } % Set sfcode to normal for the chars that usually have another value. % Can't use plain's \frenchspacing because it uses the `\x notation, and % sometimes \x has an active definition that messes things up. % \catcode`@=11 \def\plainfrenchspacing{% \sfcode`\.=\@m \sfcode`\?=\@m \sfcode`\!=\@m \sfcode`\:=\@m \sfcode`\;=\@m \sfcode`\,=\@m \def\endofsentencespacefactor{1000}% for @. and friends } \def\plainnonfrenchspacing{% \sfcode`\.3000\sfcode`\?3000\sfcode`\!3000 \sfcode`\:2000\sfcode`\;1500\sfcode`\,1250 \def\endofsentencespacefactor{3000}% for @. and friends } \catcode`@=\other \def\endofsentencespacefactor{3000}% default % @t, explicit typewriter. \def\t#1{% {\tt \rawbackslash \plainfrenchspacing #1}% \null } % @samp. \def\samp#1{{\setupmarkupstyle{samp}\lq\tclose{#1}\rq\null}} % @indicateurl is \samp, that is, with quotes. \let\indicateurl=\samp % @code (and similar) prints in typewriter, but with spaces the same % size as normal in the surrounding text, without hyphenation, etc. % This is a subroutine for that. \def\tclose#1{% {% % Change normal interword space to be same as for the current font. \spaceskip = \fontdimen2\font % % Switch to typewriter. \tt % % But `\ ' produces the large typewriter interword space. \def\ {{\spaceskip = 0pt{} }}% % % Turn off hyphenation. \nohyphenation % \rawbackslash \plainfrenchspacing #1% }% \null % reset spacefactor to 1000 } % We *must* turn on hyphenation at `-' and `_' in @code. % (But see \codedashfinish below.) % Otherwise, it is too hard to avoid overfull hboxes % in the Emacs manual, the Library manual, etc. % % Unfortunately, TeX uses one parameter (\hyphenchar) to control % both hyphenation at - and hyphenation within words. % We must therefore turn them both off (\tclose does that) % and arrange explicitly to hyphenate at a dash. -- rms. { \catcode`\-=\active \catcode`\_=\active \catcode`\'=\active \catcode`\`=\active \global\let'=\rq \global\let`=\lq % default definitions % \global\def\code{\begingroup \setupmarkupstyle{code}% % The following should really be moved into \setupmarkupstyle handlers. \catcode\dashChar=\active \catcode\underChar=\active \ifallowcodebreaks \let-\codedash \let_\codeunder \else \let-\normaldash \let_\realunder \fi % Given -foo (with a single dash), we do not want to allow a break % after the hyphen. \global\let\codedashprev=\codedash % \codex } % \gdef\codedash{\futurelet\next\codedashfinish} \gdef\codedashfinish{% \normaldash % always output the dash character itself. % % Now, output a discretionary to allow a line break, unless % (a) the next character is a -, or % (b) the preceding character is a -. % E.g., given --posix, we do not want to allow a break after either -. % Given --foo-bar, we do want to allow a break between the - and the b. \ifx\next\codedash \else \ifx\codedashprev\codedash \else \discretionary{}{}{}\fi \fi % we need the space after the = for the case when \next itself is a % space token; it would get swallowed otherwise. As in @code{- a}. \global\let\codedashprev= \next } } \def\normaldash{-} % \def\codex #1{\tclose{#1}\endgroup} \def\codeunder{% % this is all so @math{@code{var_name}+1} can work. In math mode, _ % is "active" (mathcode"8000) and \normalunderscore (or \char95, etc.) % will therefore expand the active definition of _, which is us % (inside @code that is), therefore an endless loop. \ifusingtt{\ifmmode \mathchar"075F % class 0=ordinary, family 7=ttfam, pos 0x5F=_. \else\normalunderscore \fi \discretionary{}{}{}}% {\_}% } % An additional complication: the above will allow breaks after, e.g., % each of the four underscores in __typeof__. This is bad. % @allowcodebreaks provides a document-level way to turn breaking at - % and _ on and off. % \newif\ifallowcodebreaks \allowcodebreakstrue \def\keywordtrue{true} \def\keywordfalse{false} \parseargdef\allowcodebreaks{% \def\txiarg{#1}% \ifx\txiarg\keywordtrue \allowcodebreakstrue \else\ifx\txiarg\keywordfalse \allowcodebreaksfalse \else \errhelp = \EMsimple \errmessage{Unknown @allowcodebreaks option `\txiarg', must be true|false}% \fi\fi } % For @command, @env, @file, @option quotes seem unnecessary, % so use \code rather than \samp. \let\command=\code \let\env=\code \let\file=\code \let\option=\code % @uref (abbreviation for `urlref') aka @url takes an optional % (comma-separated) second argument specifying the text to display and % an optional third arg as text to display instead of (rather than in % addition to) the url itself. First (mandatory) arg is the url. % TeX-only option to allow changing PDF output to show only the second % arg (if given), and not the url (which is then just the link target). \newif\ifurefurlonlylink % The main macro is \urefbreak, which allows breaking at expected % places within the url. (There used to be another version, which % didn't support automatic breaking.) \def\urefbreak{\begingroup \urefcatcodes \dourefbreak} \let\uref=\urefbreak % \def\dourefbreak#1{\urefbreakfinish #1,,,\finish} \def\urefbreakfinish#1,#2,#3,#4\finish{% doesn't work in @example \unsepspaces \pdfurl{#1}% \setbox0 = \hbox{\ignorespaces #3}% \ifdim\wd0 > 0pt \unhbox0 % third arg given, show only that \else \setbox0 = \hbox{\ignorespaces #2}% look for second arg \ifdim\wd0 > 0pt \ifpdf % For pdfTeX and LuaTeX \ifurefurlonlylink % PDF plus option to not display url, show just arg \unhbox0 \else % PDF, normally display both arg and url for consistency, % visibility, if the pdf is eventually used to print, etc. \unhbox0\ (\urefcode{#1})% \fi \else \ifx\XeTeXrevision\thisisundefined \unhbox0\ (\urefcode{#1})% DVI, always show arg and url \else % For XeTeX \ifurefurlonlylink % PDF plus option to not display url, show just arg \unhbox0 \else % PDF, normally display both arg and url for consistency, % visibility, if the pdf is eventually used to print, etc. \unhbox0\ (\urefcode{#1})% \fi \fi \fi \else \urefcode{#1}% only url given, so show it \fi \fi \endlink \endgroup} % Allow line breaks around only a few characters (only). \def\urefcatcodes{% \catcode`\&=\active \catcode`\.=\active \catcode`\#=\active \catcode`\?=\active \catcode`\/=\active } { \urefcatcodes % \global\def\urefcode{\begingroup \setupmarkupstyle{code}% \urefcatcodes \let&\urefcodeamp \let.\urefcodedot \let#\urefcodehash \let?\urefcodequest \let/\urefcodeslash \codex } % % By default, they are just regular characters. \global\def&{\normalamp} \global\def.{\normaldot} \global\def#{\normalhash} \global\def?{\normalquest} \global\def/{\normalslash} } % we put a little stretch before and after the breakable chars, to help % line breaking of long url's. The unequal skips make look better in % cmtt at least, especially for dots. \def\urefprestretchamount{.13em} \def\urefpoststretchamount{.1em} \def\urefprestretch{\urefprebreak \hskip0pt plus\urefprestretchamount\relax} \def\urefpoststretch{\urefpostbreak \hskip0pt plus\urefprestretchamount\relax} % \def\urefcodeamp{\urefprestretch \&\urefpoststretch} \def\urefcodedot{\urefprestretch .\urefpoststretch} \def\urefcodehash{\urefprestretch \#\urefpoststretch} \def\urefcodequest{\urefprestretch ?\urefpoststretch} \def\urefcodeslash{\futurelet\next\urefcodeslashfinish} { \catcode`\/=\active \global\def\urefcodeslashfinish{% \urefprestretch \slashChar % Allow line break only after the final / in a sequence of % slashes, to avoid line break between the slashes in http://. \ifx\next/\else \urefpoststretch \fi } } % One more complication: by default we'll break after the special % characters, but some people like to break before the special chars, so % allow that. Also allow no breaking at all, for manual control. % \parseargdef\urefbreakstyle{% \def\txiarg{#1}% \ifx\txiarg\wordnone \def\urefprebreak{\nobreak}\def\urefpostbreak{\nobreak} \else\ifx\txiarg\wordbefore \def\urefprebreak{\allowbreak}\def\urefpostbreak{\nobreak} \else\ifx\txiarg\wordafter \def\urefprebreak{\nobreak}\def\urefpostbreak{\allowbreak} \else \errhelp = \EMsimple \errmessage{Unknown @urefbreakstyle setting `\txiarg'}% \fi\fi\fi } \def\wordafter{after} \def\wordbefore{before} \def\wordnone{none} \urefbreakstyle after % @url synonym for @uref, since that's how everyone uses it. % \let\url=\uref % rms does not like angle brackets --karl, 17may97. % So now @email is just like @uref, unless we are pdf. % %\def\email#1{\angleleft{\tt #1}\angleright} \ifpdf \def\email#1{\doemail#1,,\finish} \def\doemail#1,#2,#3\finish{\begingroup \unsepspaces \pdfurl{mailto:#1}% \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0>0pt\unhbox0\else\code{#1}\fi \endlink \endgroup} \else \ifx\XeTeXrevision\thisisundefined \let\email=\uref \else \def\email#1{\doemail#1,,\finish} \def\doemail#1,#2,#3\finish{\begingroup \unsepspaces \pdfurl{mailto:#1}% \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0>0pt\unhbox0\else\code{#1}\fi \endlink \endgroup} \fi \fi % @kbdinputstyle -- arg is `distinct' (@kbd uses slanted tty font always), % `example' (@kbd uses ttsl only inside of @example and friends), % or `code' (@kbd uses normal tty font always). \parseargdef\kbdinputstyle{% \def\txiarg{#1}% \ifx\txiarg\worddistinct \gdef\kbdexamplefont{\ttsl}\gdef\kbdfont{\ttsl}% \else\ifx\txiarg\wordexample \gdef\kbdexamplefont{\ttsl}\gdef\kbdfont{\tt}% \else\ifx\txiarg\wordcode \gdef\kbdexamplefont{\tt}\gdef\kbdfont{\tt}% \else \errhelp = \EMsimple \errmessage{Unknown @kbdinputstyle setting `\txiarg'}% \fi\fi\fi } \def\worddistinct{distinct} \def\wordexample{example} \def\wordcode{code} % Default is `distinct'. \kbdinputstyle distinct % @kbd is like @code, except that if the argument is just one @key command, % then @kbd has no effect. \def\kbd#1{{\def\look{#1}\expandafter\kbdsub\look??\par}} \def\xkey{\key} \def\kbdsub#1#2#3\par{% \def\one{#1}\def\three{#3}\def\threex{??}% \ifx\one\xkey\ifx\threex\three \key{#2}% \else{\tclose{\kbdfont\setupmarkupstyle{kbd}\look}}\fi \else{\tclose{\kbdfont\setupmarkupstyle{kbd}\look}}\fi } % definition of @key that produces a lozenge. Doesn't adjust to text size. %\setfont\keyrm\rmshape{8}{1000}{OT1} %\font\keysy=cmsy9 %\def\key#1{{\keyrm\textfont2=\keysy \leavevmode\hbox{% % \raise0.4pt\hbox{\angleleft}\kern-.08em\vtop{% % \vbox{\hrule\kern-0.4pt % \hbox{\raise0.4pt\hbox{\vphantom{\angleleft}}#1}}% % \kern-0.4pt\hrule}% % \kern-.06em\raise0.4pt\hbox{\angleright}}}} % definition of @key with no lozenge. If the current font is already % monospace, don't change it; that way, we respect @kbdinputstyle. But % if it isn't monospace, then use \tt. % \def\key#1{{\setupmarkupstyle{key}% \nohyphenation \ifmonospace\else\tt\fi #1}\null} % @clicksequence{File @click{} Open ...} \def\clicksequence#1{\begingroup #1\endgroup} % @clickstyle @arrow (by default) \parseargdef\clickstyle{\def\click{#1}} \def\click{\arrow} % Typeset a dimension, e.g., `in' or `pt'. The only reason for the % argument is to make the input look right: @dmn{pt} instead of @dmn{}pt. % \def\dmn#1{\thinspace #1} % @acronym for "FBI", "NATO", and the like. % We print this one point size smaller, since it's intended for % all-uppercase. % \def\acronym#1{\doacronym #1,,\finish} \def\doacronym#1,#2,#3\finish{% {\switchtolsize #1}% \def\temp{#2}% \ifx\temp\empty \else \space ({\unsepspaces \ignorespaces \temp \unskip})% \fi \null % reset \spacefactor=1000 } % @abbr for "Comput. J." and the like. % No font change, but don't do end-of-sentence spacing. % \def\abbr#1{\doabbr #1,,\finish} \def\doabbr#1,#2,#3\finish{% {\plainfrenchspacing #1}% \def\temp{#2}% \ifx\temp\empty \else \space ({\unsepspaces \ignorespaces \temp \unskip})% \fi \null % reset \spacefactor=1000 } % @asis just yields its argument. Used with @table, for example. % \def\asis#1{#1} % @math outputs its argument in math mode. % % One complication: _ usually means subscripts, but it could also mean % an actual _ character, as in @math{@var{some_variable} + 1}. So make % _ active, and distinguish by seeing if the current family is \slfam, % which is what @var uses. { \catcode`\_ = \active \gdef\mathunderscore{% \catcode`\_=\active \def_{\ifnum\fam=\slfam \_\else\sb\fi}% } } % Another complication: we want \\ (and @\) to output a math (or tt) \. % FYI, plain.tex uses \\ as a temporary control sequence (for no % particular reason), but this is not advertised and we don't care. % % The \mathchar is class=0=ordinary, family=7=ttfam, position=5C=\. \def\mathbackslash{\ifnum\fam=\ttfam \mathchar"075C \else\backslash \fi} % \def\math{% \ifmmode\else % only go into math if not in math mode already \tex \mathunderscore \let\\ = \mathbackslash \mathactive % make the texinfo accent commands work in math mode \let\"=\ddot \let\'=\acute \let\==\bar \let\^=\hat \let\`=\grave \let\u=\breve \let\v=\check \let\~=\tilde \let\dotaccent=\dot % have to provide another name for sup operator \let\mathopsup=\sup $\expandafter\finishmath\fi } \def\finishmath#1{#1$\endgroup} % Close the group opened by \tex. % Some active characters (such as <) are spaced differently in math. % We have to reset their definitions in case the @math was an argument % to a command which sets the catcodes (such as @item or @section). % { \catcode`^ = \active \catcode`< = \active \catcode`> = \active \catcode`+ = \active \catcode`' = \active \gdef\mathactive{% \let^ = \ptexhat \let< = \ptexless \let> = \ptexgtr \let+ = \ptexplus \let' = \ptexquoteright } } % for @sub and @sup, if in math mode, just do a normal sub/superscript. % If in text, use math to place as sub/superscript, but switch % into text mode, with smaller fonts. This is a different font than the % one used for real math sub/superscripts (8pt vs. 7pt), but let's not % fix it (significant additions to font machinery) until someone notices. % \def\sub{\ifmmode \expandafter\sb \else \expandafter\finishsub\fi} \def\finishsub#1{$\sb{\hbox{\switchtolllsize #1}}$}% % \def\sup{\ifmmode \expandafter\ptexsp \else \expandafter\finishsup\fi} \def\finishsup#1{$\ptexsp{\hbox{\switchtolllsize #1}}$}% % @inlinefmt{FMTNAME,PROCESSED-TEXT} and @inlineraw{FMTNAME,RAW-TEXT}. % Ignore unless FMTNAME == tex; then it is like @iftex and @tex, % except specified as a normal braced arg, so no newlines to worry about. % \def\outfmtnametex{tex} % \long\def\inlinefmt#1{\doinlinefmt #1,\finish} \long\def\doinlinefmt#1,#2,\finish{% \def\inlinefmtname{#1}% \ifx\inlinefmtname\outfmtnametex \ignorespaces #2\fi } % % @inlinefmtifelse{FMTNAME,THEN-TEXT,ELSE-TEXT} expands THEN-TEXT if % FMTNAME is tex, else ELSE-TEXT. \long\def\inlinefmtifelse#1{\doinlinefmtifelse #1,,,\finish} \long\def\doinlinefmtifelse#1,#2,#3,#4,\finish{% \def\inlinefmtname{#1}% \ifx\inlinefmtname\outfmtnametex \ignorespaces #2\else \ignorespaces #3\fi } % % For raw, must switch into @tex before parsing the argument, to avoid % setting catcodes prematurely. Doing it this way means that, for % example, @inlineraw{html, foo{bar} gets a parse error instead of being % ignored. But this isn't important because if people want a literal % *right* brace they would have to use a command anyway, so they may as % well use a command to get a left brace too. We could re-use the % delimiter character idea from \verb, but it seems like overkill. % \long\def\inlineraw{\tex \doinlineraw} \long\def\doinlineraw#1{\doinlinerawtwo #1,\finish} \def\doinlinerawtwo#1,#2,\finish{% \def\inlinerawname{#1}% \ifx\inlinerawname\outfmtnametex \ignorespaces #2\fi \endgroup % close group opened by \tex. } % @inlineifset{VAR, TEXT} expands TEXT if VAR is @set. % \long\def\inlineifset#1{\doinlineifset #1,\finish} \long\def\doinlineifset#1,#2,\finish{% \def\inlinevarname{#1}% \expandafter\ifx\csname SET\inlinevarname\endcsname\relax \else\ignorespaces#2\fi } % @inlineifclear{VAR, TEXT} expands TEXT if VAR is not @set. % \long\def\inlineifclear#1{\doinlineifclear #1,\finish} \long\def\doinlineifclear#1,#2,\finish{% \def\inlinevarname{#1}% \expandafter\ifx\csname SET\inlinevarname\endcsname\relax \ignorespaces#2\fi } \message{glyphs,} % and logos. % @@ prints an @, as does @atchar{}. \def\@{\char64 } \let\atchar=\@ % @{ @} @lbracechar{} @rbracechar{} all generate brace characters. \def\lbracechar{{\ifmonospace\char123\else\ensuremath\lbrace\fi}} \def\rbracechar{{\ifmonospace\char125\else\ensuremath\rbrace\fi}} \let\{=\lbracechar \let\}=\rbracechar % @comma{} to avoid , parsing problems. \let\comma = , % Accents: @, @dotaccent @ringaccent @ubaraccent @udotaccent % Others are defined by plain TeX: @` @' @" @^ @~ @= @u @v @H. \let\, = \ptexc \let\dotaccent = \ptexdot \def\ringaccent#1{{\accent23 #1}} \let\tieaccent = \ptext \let\ubaraccent = \ptexb \let\udotaccent = \d % Other special characters: @questiondown @exclamdown @ordf @ordm % Plain TeX defines: @AA @AE @O @OE @L (plus lowercase versions) @ss. \def\questiondown{?`} \def\exclamdown{!`} \def\ordf{\leavevmode\raise1ex\hbox{\switchtolllsize \underbar{a}}} \def\ordm{\leavevmode\raise1ex\hbox{\switchtolllsize \underbar{o}}} % Dotless i and dotless j, used for accents. \def\imacro{i} \def\jmacro{j} \def\dotless#1{% \def\temp{#1}% \ifx\temp\imacro \ifmmode\imath \else\ptexi \fi \else\ifx\temp\jmacro \ifmmode\jmath \else\j \fi \else \errmessage{@dotless can be used only with i or j}% \fi\fi } % The \TeX{} logo, as in plain, but resetting the spacing so that a % period following counts as ending a sentence. (Idea found in latex.) % \edef\TeX{\TeX \spacefactor=1000 } % @LaTeX{} logo. Not quite the same results as the definition in % latex.ltx, since we use a different font for the raised A; it's most % convenient for us to use an explicitly smaller font, rather than using % the \scriptstyle font (since we don't reset \scriptstyle and % \scriptscriptstyle). % \def\LaTeX{% L\kern-.36em {\setbox0=\hbox{T}% \vbox to \ht0{\hbox{% \ifx\textnominalsize\xwordpt % for 10pt running text, lllsize (8pt) is too small for the A in LaTeX. % Revert to plain's \scriptsize, which is 7pt. \count255=\the\fam $\fam\count255 \scriptstyle A$% \else % For 11pt, we can use our lllsize. \switchtolllsize A% \fi }% \vss }}% \kern-.15em \TeX } % Some math mode symbols. Define \ensuremath to switch into math mode % unless we are already there. Expansion tricks may not be needed here, % but safer, and can't hurt. \def\ensuremath{\ifmmode \expandafter\asis \else\expandafter\ensuredmath \fi} \def\ensuredmath#1{$\relax#1$} % \def\bullet{\ensuremath\ptexbullet} \def\geq{\ensuremath\ge} \def\leq{\ensuremath\le} \def\minus{\ensuremath-} % @dots{} outputs an ellipsis using the current font. % We do .5em per period so that it has the same spacing in the cm % typewriter fonts as three actual period characters; on the other hand, % in other typewriter fonts three periods are wider than 1.5em. So do % whichever is larger. % \def\dots{% \leavevmode \setbox0=\hbox{...}% get width of three periods \ifdim\wd0 > 1.5em \dimen0 = \wd0 \else \dimen0 = 1.5em \fi \hbox to \dimen0{% \hskip 0pt plus.25fil .\hskip 0pt plus1fil .\hskip 0pt plus1fil .\hskip 0pt plus.5fil }% } % @enddots{} is an end-of-sentence ellipsis. % \def\enddots{% \dots \spacefactor=\endofsentencespacefactor } % @point{}, @result{}, @expansion{}, @print{}, @equiv{}. % % Since these characters are used in examples, they should be an even number of % \tt widths. Each \tt character is 1en, so two makes it 1em. % \def\point{$\star$} \def\arrow{\leavevmode\raise.05ex\hbox to 1em{\hfil$\rightarrow$\hfil}} \def\result{\leavevmode\raise.05ex\hbox to 1em{\hfil$\Rightarrow$\hfil}} \def\expansion{\leavevmode\hbox to 1em{\hfil$\mapsto$\hfil}} \def\print{\leavevmode\lower.1ex\hbox to 1em{\hfil$\dashv$\hfil}} \def\equiv{\leavevmode\hbox to 1em{\hfil$\ptexequiv$\hfil}} % The @error{} command. % Adapted from the TeXbook's \boxit. % \newbox\errorbox % {\ttfont \global\dimen0 = 3em}% Width of the box. \dimen2 = .55pt % Thickness of rules % The text. (`r' is open on the right, `e' somewhat less so on the left.) \setbox0 = \hbox{\kern-.75pt \reducedsf \putworderror\kern-1.5pt} % \setbox\errorbox=\hbox to \dimen0{\hfil \hsize = \dimen0 \advance\hsize by -5.8pt % Space to left+right. \advance\hsize by -2\dimen2 % Rules. \vbox{% \hrule height\dimen2 \hbox{\vrule width\dimen2 \kern3pt % Space to left of text. \vtop{\kern2.4pt \box0 \kern2.4pt}% Space above/below. \kern3pt\vrule width\dimen2}% Space to right. \hrule height\dimen2} \hfil} % \def\error{\leavevmode\lower.7ex\copy\errorbox} % @pounds{} is a sterling sign, which Knuth put in the CM italic font. % \def\pounds{{\it\$}} % @euro{} comes from a separate font, depending on the current style. % We use the free feym* fonts from the eurosym package by Henrik % Theiling, which support regular, slanted, bold and bold slanted (and % "outlined" (blackboard board, sort of) versions, which we don't need). % It is available from http://www.ctan.org/tex-archive/fonts/eurosym. % % Although only regular is the truly official Euro symbol, we ignore % that. The Euro is designed to be slightly taller than the regular % font height. % % feymr - regular % feymo - slanted % feybr - bold % feybo - bold slanted % % There is no good (free) typewriter version, to my knowledge. % A feymr10 euro is ~7.3pt wide, while a normal cmtt10 char is ~5.25pt wide. % Hmm. % % Also doesn't work in math. Do we need to do math with euro symbols? % Hope not. % % \def\euro{{\eurofont e}} \def\eurofont{% % We set the font at each command, rather than predefining it in % \textfonts and the other font-switching commands, so that % installations which never need the symbol don't have to have the % font installed. % % There is only one designed size (nominal 10pt), so we always scale % that to the current nominal size. % % By the way, simply using "at 1em" works for cmr10 and the like, but % does not work for cmbx10 and other extended/shrunken fonts. % \def\eurosize{\csname\curfontsize nominalsize\endcsname}% % \ifx\curfontstyle\bfstylename % bold: \font\thiseurofont = \ifusingit{feybo10}{feybr10} at \eurosize \else % regular: \font\thiseurofont = \ifusingit{feymo10}{feymr10} at \eurosize \fi \thiseurofont } % Glyphs from the EC fonts. We don't use \let for the aliases, because % sometimes we redefine the original macro, and the alias should reflect % the redefinition. % % Use LaTeX names for the Icelandic letters. \def\DH{{\ecfont \char"D0}} % Eth \def\dh{{\ecfont \char"F0}} % eth \def\TH{{\ecfont \char"DE}} % Thorn \def\th{{\ecfont \char"FE}} % thorn % \def\guillemetleft{{\ecfont \char"13}} \def\guillemotleft{\guillemetleft} \def\guillemetright{{\ecfont \char"14}} \def\guillemotright{\guillemetright} \def\guilsinglleft{{\ecfont \char"0E}} \def\guilsinglright{{\ecfont \char"0F}} \def\quotedblbase{{\ecfont \char"12}} \def\quotesinglbase{{\ecfont \char"0D}} % % This positioning is not perfect (see the ogonek LaTeX package), but % we have the precomposed glyphs for the most common cases. We put the % tests to use those glyphs in the single \ogonek macro so we have fewer % dummy definitions to worry about for index entries, etc. % % ogonek is also used with other letters in Lithuanian (IOU), but using % the precomposed glyphs for those is not so easy since they aren't in % the same EC font. \def\ogonek#1{{% \def\temp{#1}% \ifx\temp\macrocharA\Aogonek \else\ifx\temp\macrochara\aogonek \else\ifx\temp\macrocharE\Eogonek \else\ifx\temp\macrochare\eogonek \else \ecfont \setbox0=\hbox{#1}% \ifdim\ht0=1ex\accent"0C #1% \else\ooalign{\unhbox0\crcr\hidewidth\char"0C \hidewidth}% \fi \fi\fi\fi\fi }% } \def\Aogonek{{\ecfont \char"81}}\def\macrocharA{A} \def\aogonek{{\ecfont \char"A1}}\def\macrochara{a} \def\Eogonek{{\ecfont \char"86}}\def\macrocharE{E} \def\eogonek{{\ecfont \char"A6}}\def\macrochare{e} % % Use the European Computer Modern fonts (cm-super in outline format) % for non-CM glyphs. That is ec* for regular text and tc* for the text % companion symbols (LaTeX TS1 encoding). Both are part of the ec % package and follow the same conventions. % \def\ecfont{\etcfont{e}} \def\tcfont{\etcfont{t}} % \def\etcfont#1{% % We can't distinguish serif/sans and italic/slanted, but this % is used for crude hacks anyway (like adding French and German % quotes to documents typeset with CM, where we lose kerning), so % hopefully nobody will notice/care. \edef\ecsize{\csname\curfontsize ecsize\endcsname}% \edef\nominalsize{\csname\curfontsize nominalsize\endcsname}% \ifmonospace % typewriter: \font\thisecfont = #1ctt\ecsize \space at \nominalsize \else \ifx\curfontstyle\bfstylename % bold: \font\thisecfont = #1cb\ifusingit{i}{x}\ecsize \space at \nominalsize \else % regular: \font\thisecfont = #1c\ifusingit{ti}{rm}\ecsize \space at \nominalsize \fi \fi \thisecfont } % @registeredsymbol - R in a circle. The font for the R should really % be smaller yet, but lllsize is the best we can do for now. % Adapted from the plain.tex definition of \copyright. % \def\registeredsymbol{% $^{{\ooalign{\hfil\raise.07ex\hbox{\switchtolllsize R}% \hfil\crcr\Orb}}% }$% } % @textdegree - the normal degrees sign. % \def\textdegree{$^\circ$} % Laurent Siebenmann reports \Orb undefined with: % Textures 1.7.7 (preloaded format=plain 93.10.14) (68K) 16 APR 2004 02:38 % so we'll define it if necessary. % \ifx\Orb\thisisundefined \def\Orb{\mathhexbox20D} \fi % Quotes. \chardef\quotedblleft="5C \chardef\quotedblright=`\" \chardef\quoteleft=`\` \chardef\quoteright=`\' \message{page headings,} \newskip\titlepagetopglue \titlepagetopglue = 1.5in \newskip\titlepagebottomglue \titlepagebottomglue = 2pc % First the title page. Must do @settitle before @titlepage. \newif\ifseenauthor \newif\iffinishedtitlepage % @setcontentsaftertitlepage used to do an implicit @contents or % @shortcontents after @end titlepage, but it is now obsolete. \def\setcontentsaftertitlepage{% \errmessage{@setcontentsaftertitlepage has been removed as a Texinfo command; move your @contents command if you want the contents after the title page.}}% \def\setshortcontentsaftertitlepage{% \errmessage{@setshortcontentsaftertitlepage has been removed as a Texinfo command; move your @shortcontents and @contents commands if you want the contents after the title page.}}% \parseargdef\shorttitlepage{% \begingroup \hbox{}\vskip 1.5in \chaprm \centerline{#1}% \endgroup\page\hbox{}\page} \envdef\titlepage{% % Open one extra group, as we want to close it in the middle of \Etitlepage. \begingroup \parindent=0pt \textfonts % Leave some space at the very top of the page. \vglue\titlepagetopglue % No rule at page bottom unless we print one at the top with @title. \finishedtitlepagetrue % % Most title ``pages'' are actually two pages long, with space % at the top of the second. We don't want the ragged left on the second. \let\oldpage = \page \def\page{% \iffinishedtitlepage\else \finishtitlepage \fi \let\page = \oldpage \page \null }% } \def\Etitlepage{% \iffinishedtitlepage\else \finishtitlepage \fi % It is important to do the page break before ending the group, % because the headline and footline are only empty inside the group. % If we use the new definition of \page, we always get a blank page % after the title page, which we certainly don't want. \oldpage \endgroup % % Need this before the \...aftertitlepage checks so that if they are % in effect the toc pages will come out with page numbers. \HEADINGSon } \def\finishtitlepage{% \vskip4pt \hrule height 2pt width \hsize \vskip\titlepagebottomglue \finishedtitlepagetrue } % Settings used for typesetting titles: no hyphenation, no indentation, % don't worry much about spacing, ragged right. This should be used % inside a \vbox, and fonts need to be set appropriately first. \par should % be specified before the end of the \vbox, since a vbox is a group. % \def\raggedtitlesettings{% \rm \hyphenpenalty=10000 \parindent=0pt \tolerance=5000 \ptexraggedright } % Macros to be used within @titlepage: \let\subtitlerm=\rmfont \def\subtitlefont{\subtitlerm \normalbaselineskip = 13pt \normalbaselines} \parseargdef\title{% \checkenv\titlepage \vbox{\titlefonts \raggedtitlesettings #1\par}% % print a rule at the page bottom also. \finishedtitlepagefalse \vskip4pt \hrule height 4pt width \hsize \vskip4pt } \parseargdef\subtitle{% \checkenv\titlepage {\subtitlefont \rightline{#1}}% } % @author should come last, but may come many times. % It can also be used inside @quotation. % \parseargdef\author{% \def\temp{\quotation}% \ifx\thisenv\temp \def\quotationauthor{#1}% printed in \Equotation. \else \checkenv\titlepage \ifseenauthor\else \vskip 0pt plus 1filll \seenauthortrue \fi {\secfonts\rm \leftline{#1}}% \fi } % Set up page headings and footings. \let\thispage=\folio \newtoks\evenheadline % headline on even pages \newtoks\oddheadline % headline on odd pages \newtoks\evenfootline % footline on even pages \newtoks\oddfootline % footline on odd pages % Now make \makeheadline and \makefootline in Plain TeX use those variables \headline={{\textfonts\rm \ifodd\pageno \the\oddheadline \else \the\evenheadline \fi}} \footline={{\textfonts\rm \ifodd\pageno \the\oddfootline \else \the\evenfootline \fi}\HEADINGShook} \let\HEADINGShook=\relax % Commands to set those variables. % For example, this is what @headings on does % @evenheading @thistitle|@thispage|@thischapter % @oddheading @thischapter|@thispage|@thistitle % @evenfooting @thisfile|| % @oddfooting ||@thisfile \def\evenheading{\parsearg\evenheadingxxx} \def\evenheadingxxx #1{\evenheadingyyy #1\|\|\|\|\finish} \def\evenheadingyyy #1\|#2\|#3\|#4\finish{% \global\evenheadline={\rlap{\centerline{#2}}\line{#1\hfil#3}}} \def\oddheading{\parsearg\oddheadingxxx} \def\oddheadingxxx #1{\oddheadingyyy #1\|\|\|\|\finish} \def\oddheadingyyy #1\|#2\|#3\|#4\finish{% \global\oddheadline={\rlap{\centerline{#2}}\line{#1\hfil#3}}} \parseargdef\everyheading{\oddheadingxxx{#1}\evenheadingxxx{#1}}% \def\evenfooting{\parsearg\evenfootingxxx} \def\evenfootingxxx #1{\evenfootingyyy #1\|\|\|\|\finish} \def\evenfootingyyy #1\|#2\|#3\|#4\finish{% \global\evenfootline={\rlap{\centerline{#2}}\line{#1\hfil#3}}} \def\oddfooting{\parsearg\oddfootingxxx} \def\oddfootingxxx #1{\oddfootingyyy #1\|\|\|\|\finish} \def\oddfootingyyy #1\|#2\|#3\|#4\finish{% \global\oddfootline = {\rlap{\centerline{#2}}\line{#1\hfil#3}}% % % Leave some space for the footline. Hopefully ok to assume % @evenfooting will not be used by itself. \global\advance\txipageheight by -12pt \global\advance\vsize by -12pt } \parseargdef\everyfooting{\oddfootingxxx{#1}\evenfootingxxx{#1}} % @evenheadingmarks top \thischapter <- chapter at the top of a page % @evenheadingmarks bottom \thischapter <- chapter at the bottom of a page % % The same set of arguments for: % % @oddheadingmarks % @evenfootingmarks % @oddfootingmarks % @everyheadingmarks % @everyfootingmarks % These define \getoddheadingmarks, \getevenheadingmarks, % \getoddfootingmarks, and \getevenfootingmarks, each to one of % \gettopheadingmarks, \getbottomheadingmarks. % \def\evenheadingmarks{\headingmarks{even}{heading}} \def\oddheadingmarks{\headingmarks{odd}{heading}} \def\evenfootingmarks{\headingmarks{even}{footing}} \def\oddfootingmarks{\headingmarks{odd}{footing}} \parseargdef\everyheadingmarks{\headingmarks{even}{heading}{#1} \headingmarks{odd}{heading}{#1} } \parseargdef\everyfootingmarks{\headingmarks{even}{footing}{#1} \headingmarks{odd}{footing}{#1} } % #1 = even/odd, #2 = heading/footing, #3 = top/bottom. \def\headingmarks#1#2#3 {% \expandafter\let\expandafter\temp \csname get#3headingmarks\endcsname \global\expandafter\let\csname get#1#2marks\endcsname \temp } \everyheadingmarks bottom \everyfootingmarks bottom % @headings double turns headings on for double-sided printing. % @headings single turns headings on for single-sided printing. % @headings off turns them off. % @headings on same as @headings double, retained for compatibility. % @headings after turns on double-sided headings after this page. % @headings doubleafter turns on double-sided headings after this page. % @headings singleafter turns on single-sided headings after this page. % By default, they are off at the start of a document, % and turned `on' after @end titlepage. \parseargdef\headings{\csname HEADINGS#1\endcsname} \def\headingsoff{% non-global headings elimination \evenheadline={\hfil}\evenfootline={\hfil}% \oddheadline={\hfil}\oddfootline={\hfil}% } \def\HEADINGSoff{{\globaldefs=1 \headingsoff}} % global setting \HEADINGSoff % it's the default % When we turn headings on, set the page number to 1. % For double-sided printing, put current file name in lower left corner, % chapter name on inside top of right hand pages, document % title on inside top of left hand pages, and page numbers on outside top % edge of all pages. \def\HEADINGSdouble{% \global\pageno=1 \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\folio\hfil\thistitle}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chapoddpage } \let\contentsalignmacro = \chappager % For single-sided printing, chapter title goes across top left of page, % page number on top right. \def\HEADINGSsingle{% \global\pageno=1 \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\thischapterheading\hfil\folio}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chappager } \def\HEADINGSon{\HEADINGSdouble} \def\HEADINGSafter{\let\HEADINGShook=\HEADINGSdoublex} \let\HEADINGSdoubleafter=\HEADINGSafter \def\HEADINGSdoublex{% \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\folio\hfil\thistitle}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chapoddpage } \def\HEADINGSsingleafter{\let\HEADINGShook=\HEADINGSsinglex} \def\HEADINGSsinglex{% \global\evenfootline={\hfil} \global\oddfootline={\hfil} \global\evenheadline={\line{\thischapterheading\hfil\folio}} \global\oddheadline={\line{\thischapterheading\hfil\folio}} \global\let\contentsalignmacro = \chappager } % Subroutines used in generating headings % This produces Day Month Year style of output. % Only define if not already defined, in case a txi-??.tex file has set % up a different format (e.g., txi-cs.tex does this). \ifx\today\thisisundefined \def\today{% \number\day\space \ifcase\month \or\putwordMJan\or\putwordMFeb\or\putwordMMar\or\putwordMApr \or\putwordMMay\or\putwordMJun\or\putwordMJul\or\putwordMAug \or\putwordMSep\or\putwordMOct\or\putwordMNov\or\putwordMDec \fi \space\number\year} \fi % @settitle line... specifies the title of the document, for headings. % It generates no output of its own. \def\thistitle{\putwordNoTitle} \def\settitle{\parsearg{\gdef\thistitle}} \message{tables,} % Tables -- @table, @ftable, @vtable, @item(x). % default indentation of table text \newdimen\tableindent \tableindent=.8in % default indentation of @itemize and @enumerate text \newdimen\itemindent \itemindent=.3in % margin between end of table item and start of table text. \newdimen\itemmargin \itemmargin=.1in % used internally for \itemindent minus \itemmargin \newdimen\itemmax % Note @table, @ftable, and @vtable define @item, @itemx, etc., with % these defs. % They also define \itemindex % to index the item name in whatever manner is desired (perhaps none). \newif\ifitemxneedsnegativevskip \def\itemxpar{\par\ifitemxneedsnegativevskip\nobreak\vskip-\parskip\nobreak\fi} \def\internalBitem{\smallbreak \parsearg\itemzzz} \def\internalBitemx{\itemxpar \parsearg\itemzzz} \def\itemzzz #1{\begingroup % \advance\hsize by -\rightskip \advance\hsize by -\tableindent \setbox0=\hbox{\itemindicate{#1}}% \itemindex{#1}% \nobreak % This prevents a break before @itemx. % % If the item text does not fit in the space we have, put it on a line % by itself, and do not allow a page break either before or after that % line. We do not start a paragraph here because then if the next % command is, e.g., @kindex, the whatsit would get put into the % horizontal list on a line by itself, resulting in extra blank space. \ifdim \wd0>\itemmax % % Make this a paragraph so we get the \parskip glue and wrapping, % but leave it ragged-right. \begingroup \advance\leftskip by-\tableindent \advance\hsize by\tableindent \advance\rightskip by0pt plus1fil\relax \leavevmode\unhbox0\par \endgroup % % We're going to be starting a paragraph, but we don't want the % \parskip glue -- logically it's part of the @item we just started. \nobreak \vskip-\parskip % % Stop a page break at the \parskip glue coming up. However, if % what follows is an environment such as @example, there will be no % \parskip glue; then the negative vskip we just inserted would % cause the example and the item to crash together. So we use this % bizarre value of 10001 as a signal to \aboveenvbreak to insert % \parskip glue after all. Section titles are handled this way also. % \penalty 10001 \endgroup \itemxneedsnegativevskipfalse \else % The item text fits into the space. Start a paragraph, so that the % following text (if any) will end up on the same line. \noindent % Do this with kerns and \unhbox so that if there is a footnote in % the item text, it can migrate to the main vertical list and % eventually be printed. \nobreak\kern-\tableindent \dimen0 = \itemmax \advance\dimen0 by \itemmargin \advance\dimen0 by -\wd0 \unhbox0 \nobreak\kern\dimen0 \endgroup \itemxneedsnegativevskiptrue \fi } \def\item{\errmessage{@item while not in a list environment}} \def\itemx{\errmessage{@itemx while not in a list environment}} % @table, @ftable, @vtable. \envdef\table{% \let\itemindex\gobble \tablecheck{table}% } \envdef\ftable{% \def\itemindex ##1{\doind {fn}{\code{##1}}}% \tablecheck{ftable}% } \envdef\vtable{% \def\itemindex ##1{\doind {vr}{\code{##1}}}% \tablecheck{vtable}% } \def\tablecheck#1{% \ifnum \the\catcode`\^^M=\active \endgroup \errmessage{This command won't work in this context; perhaps the problem is that we are \inenvironment\thisenv}% \def\next{\doignore{#1}}% \else \let\next\tablex \fi \next } \def\tablex#1{% \def\itemindicate{#1}% \parsearg\tabley } \def\tabley#1{% {% \makevalueexpandable \edef\temp{\noexpand\tablez #1\space\space\space}% \expandafter }\temp \endtablez } \def\tablez #1 #2 #3 #4\endtablez{% \aboveenvbreak \ifnum 0#1>0 \advance \leftskip by #1\mil \fi \ifnum 0#2>0 \tableindent=#2\mil \fi \ifnum 0#3>0 \advance \rightskip by #3\mil \fi \itemmax=\tableindent \advance \itemmax by -\itemmargin \advance \leftskip by \tableindent \exdentamount=\tableindent \parindent = 0pt \parskip = \smallskipamount \ifdim \parskip=0pt \parskip=2pt \fi \let\item = \internalBitem \let\itemx = \internalBitemx } \def\Etable{\endgraf\afterenvbreak} \let\Eftable\Etable \let\Evtable\Etable \let\Eitemize\Etable \let\Eenumerate\Etable % This is the counter used by @enumerate, which is really @itemize \newcount \itemno \envdef\itemize{\parsearg\doitemize} \def\doitemize#1{% \aboveenvbreak \itemmax=\itemindent \advance\itemmax by -\itemmargin \advance\leftskip by \itemindent \exdentamount=\itemindent \parindent=0pt \parskip=\smallskipamount \ifdim\parskip=0pt \parskip=2pt \fi % % Try typesetting the item mark so that if the document erroneously says % something like @itemize @samp (intending @table), there's an error % right away at the @itemize. It's not the best error message in the % world, but it's better than leaving it to the @item. This means if % the user wants an empty mark, they have to say @w{} not just @w. \def\itemcontents{#1}% \setbox0 = \hbox{\itemcontents}% % % @itemize with no arg is equivalent to @itemize @bullet. \ifx\itemcontents\empty\def\itemcontents{\bullet}\fi % \let\item=\itemizeitem } % Definition of @item while inside @itemize and @enumerate. % \def\itemizeitem{% \advance\itemno by 1 % for enumerations {\let\par=\endgraf \smallbreak}% reasonable place to break {% % If the document has an @itemize directly after a section title, a % \nobreak will be last on the list, and \sectionheading will have % done a \vskip-\parskip. In that case, we don't want to zero % parskip, or the item text will crash with the heading. On the % other hand, when there is normal text preceding the item (as there % usually is), we do want to zero parskip, or there would be too much % space. In that case, we won't have a \nobreak before. At least % that's the theory. \ifnum\lastpenalty<10000 \parskip=0in \fi \noindent \hbox to 0pt{\hss \itemcontents \kern\itemmargin}% % \ifinner\else \vadjust{\penalty 1200}% not good to break after first line of item. \fi % We can be in inner vertical mode in a footnote, although an % @itemize looks awful there. }% \flushcr } % \splitoff TOKENS\endmark defines \first to be the first token in % TOKENS, and \rest to be the remainder. % \def\splitoff#1#2\endmark{\def\first{#1}\def\rest{#2}}% % Allow an optional argument of an uppercase letter, lowercase letter, % or number, to specify the first label in the enumerated list. No % argument is the same as `1'. % \envparseargdef\enumerate{\enumeratey #1 \endenumeratey} \def\enumeratey #1 #2\endenumeratey{% % If we were given no argument, pretend we were given `1'. \def\thearg{#1}% \ifx\thearg\empty \def\thearg{1}\fi % % Detect if the argument is a single token. If so, it might be a % letter. Otherwise, the only valid thing it can be is a number. % (We will always have one token, because of the test we just made. % This is a good thing, since \splitoff doesn't work given nothing at % all -- the first parameter is undelimited.) \expandafter\splitoff\thearg\endmark \ifx\rest\empty % Only one token in the argument. It could still be anything. % A ``lowercase letter'' is one whose \lccode is nonzero. % An ``uppercase letter'' is one whose \lccode is both nonzero, and % not equal to itself. % Otherwise, we assume it's a number. % % We need the \relax at the end of the \ifnum lines to stop TeX from % continuing to look for a <number>. % \ifnum\lccode\expandafter`\thearg=0\relax \numericenumerate % a number (we hope) \else % It's a letter. \ifnum\lccode\expandafter`\thearg=\expandafter`\thearg\relax \lowercaseenumerate % lowercase letter \else \uppercaseenumerate % uppercase letter \fi \fi \else % Multiple tokens in the argument. We hope it's a number. \numericenumerate \fi } % An @enumerate whose labels are integers. The starting integer is % given in \thearg. % \def\numericenumerate{% \itemno = \thearg \startenumeration{\the\itemno}% } % The starting (lowercase) letter is in \thearg. \def\lowercaseenumerate{% \itemno = \expandafter`\thearg \startenumeration{% % Be sure we're not beyond the end of the alphabet. \ifnum\itemno=0 \errmessage{No more lowercase letters in @enumerate; get a bigger alphabet}% \fi \char\lccode\itemno }% } % The starting (uppercase) letter is in \thearg. \def\uppercaseenumerate{% \itemno = \expandafter`\thearg \startenumeration{% % Be sure we're not beyond the end of the alphabet. \ifnum\itemno=0 \errmessage{No more uppercase letters in @enumerate; get a bigger alphabet} \fi \char\uccode\itemno }% } % Call \doitemize, adding a period to the first argument and supplying the % common last two arguments. Also subtract one from the initial value in % \itemno, since @item increments \itemno. % \def\startenumeration#1{% \advance\itemno by -1 \doitemize{#1.}\flushcr } % @alphaenumerate and @capsenumerate are abbreviations for giving an arg % to @enumerate. % \def\alphaenumerate{\enumerate{a}} \def\capsenumerate{\enumerate{A}} \def\Ealphaenumerate{\Eenumerate} \def\Ecapsenumerate{\Eenumerate} % @multitable macros % Amy Hendrickson, 8/18/94, 3/6/96 % % @multitable ... @end multitable will make as many columns as desired. % Contents of each column will wrap at width given in preamble. Width % can be specified either with sample text given in a template line, % or in percent of \hsize, the current width of text on page. % Table can continue over pages but will only break between lines. % To make preamble: % % Either define widths of columns in terms of percent of \hsize: % @multitable @columnfractions .25 .3 .45 % @item ... % % Numbers following @columnfractions are the percent of the total % current hsize to be used for each column. You may use as many % columns as desired. % Or use a template: % @multitable {Column 1 template} {Column 2 template} {Column 3 template} % @item ... % using the widest term desired in each column. % Each new table line starts with @item, each subsequent new column % starts with @tab. Empty columns may be produced by supplying @tab's % with nothing between them for as many times as empty columns are needed, % ie, @tab@tab@tab will produce two empty columns. % @item, @tab do not need to be on their own lines, but it will not hurt % if they are. % Sample multitable: % @multitable {Column 1 template} {Column 2 template} {Column 3 template} % @item first col stuff @tab second col stuff @tab third col % @item % first col stuff % @tab % second col stuff % @tab % third col % @item first col stuff @tab second col stuff % @tab Many paragraphs of text may be used in any column. % % They will wrap at the width determined by the template. % @item@tab@tab This will be in third column. % @end multitable % Default dimensions may be reset by user. % @multitableparskip is vertical space between paragraphs in table. % @multitableparindent is paragraph indent in table. % @multitablecolmargin is horizontal space to be left between columns. % @multitablelinespace is space to leave between table items, baseline % to baseline. % 0pt means it depends on current normal line spacing. % \newskip\multitableparskip \newskip\multitableparindent \newdimen\multitablecolspace \newskip\multitablelinespace \multitableparskip=0pt \multitableparindent=6pt \multitablecolspace=12pt \multitablelinespace=0pt % Macros used to set up halign preamble: % \let\endsetuptable\relax \def\xendsetuptable{\endsetuptable} \let\columnfractions\relax \def\xcolumnfractions{\columnfractions} \newif\ifsetpercent % #1 is the @columnfraction, usually a decimal number like .5, but might % be just 1. We just use it, whatever it is. % \def\pickupwholefraction#1 {% \global\advance\colcount by 1 \expandafter\xdef\csname col\the\colcount\endcsname{#1\hsize}% \setuptable } \newcount\colcount \def\setuptable#1{% \def\firstarg{#1}% \ifx\firstarg\xendsetuptable \let\go = \relax \else \ifx\firstarg\xcolumnfractions \global\setpercenttrue \else \ifsetpercent \let\go\pickupwholefraction \else \global\advance\colcount by 1 \setbox0=\hbox{#1\unskip\space}% Add a normal word space as a % separator; typically that is always in the input, anyway. \expandafter\xdef\csname col\the\colcount\endcsname{\the\wd0}% \fi \fi \ifx\go\pickupwholefraction % Put the argument back for the \pickupwholefraction call, so % we'll always have a period there to be parsed. \def\go{\pickupwholefraction#1}% \else \let\go = \setuptable \fi% \fi \go } % multitable-only commands. % % @headitem starts a heading row, which we typeset in bold. Assignments % have to be global since we are inside the implicit group of an % alignment entry. \everycr below resets \everytab so we don't have to % undo it ourselves. \def\headitemfont{\b}% for people to use in the template row; not changeable \def\headitem{% \checkenv\multitable \crcr \gdef\headitemcrhook{\nobreak}% attempt to avoid page break after headings \global\everytab={\bf}% can't use \headitemfont since the parsing differs \the\everytab % for the first item }% % % default for tables with no headings. \let\headitemcrhook=\relax % % A \tab used to include \hskip1sp. But then the space in a template % line is not enough. That is bad. So let's go back to just `&' until % we again encounter the problem the 1sp was intended to solve. % --karl, nathan@acm.org, 20apr99. \def\tab{\checkenv\multitable &\the\everytab}% % @multitable ... @end multitable definitions: % \newtoks\everytab % insert after every tab. % \envdef\multitable{% \vskip\parskip \startsavinginserts % % @item within a multitable starts a normal row. % We use \def instead of \let so that if one of the multitable entries % contains an @itemize, we don't choke on the \item (seen as \crcr aka % \endtemplate) expanding \doitemize. \def\item{\crcr}% % \tolerance=9500 \hbadness=9500 \setmultitablespacing \parskip=\multitableparskip \parindent=\multitableparindent \overfullrule=0pt \global\colcount=0 % \everycr = {% \noalign{% \global\everytab={}% Reset from possible headitem. \global\colcount=0 % Reset the column counter. % % Check for saved footnotes, etc.: \checkinserts % % Perhaps a \nobreak, then reset: \headitemcrhook \global\let\headitemcrhook=\relax }% }% % \parsearg\domultitable } \def\domultitable#1{% % To parse everything between @multitable and @item: \setuptable#1 \endsetuptable % % This preamble sets up a generic column definition, which will % be used as many times as user calls for columns. % \vtop will set a single line and will also let text wrap and % continue for many paragraphs if desired. \halign\bgroup &% \global\advance\colcount by 1 \multistrut \vtop{% % Use the current \colcount to find the correct column width: \hsize=\expandafter\csname col\the\colcount\endcsname % % In order to keep entries from bumping into each other % we will add a \leftskip of \multitablecolspace to all columns after % the first one. % % If a template has been used, we will add \multitablecolspace % to the width of each template entry. % % If the user has set preamble in terms of percent of \hsize we will % use that dimension as the width of the column, and the \leftskip % will keep entries from bumping into each other. Table will start at % left margin and final column will justify at right margin. % % Make sure we don't inherit \rightskip from the outer environment. \rightskip=0pt \ifnum\colcount=1 % The first column will be indented with the surrounding text. \advance\hsize by\leftskip \else \ifsetpercent \else % If user has not set preamble in terms of percent of \hsize % we will advance \hsize by \multitablecolspace. \advance\hsize by \multitablecolspace \fi % In either case we will make \leftskip=\multitablecolspace: \leftskip=\multitablecolspace \fi % Ignoring space at the beginning and end avoids an occasional spurious % blank line, when TeX decides to break the line at the space before the % box from the multistrut, so the strut ends up on a line by itself. % For example: % @multitable @columnfractions .11 .89 % @item @code{#} % @tab Legal holiday which is valid in major parts of the whole country. % Is automatically provided with highlighting sequences respectively % marking characters. \noindent\ignorespaces##\unskip\multistrut }\cr } \def\Emultitable{% \crcr \egroup % end the \halign \global\setpercentfalse } \def\setmultitablespacing{% \def\multistrut{\strut}% just use the standard line spacing % % Compute \multitablelinespace (if not defined by user) for use in % \multitableparskip calculation. We used define \multistrut based on % this, but (ironically) that caused the spacing to be off. % See bug-texinfo report from Werner Lemberg, 31 Oct 2004 12:52:20 +0100. \ifdim\multitablelinespace=0pt \setbox0=\vbox{X}\global\multitablelinespace=\the\baselineskip \global\advance\multitablelinespace by-\ht0 \fi % Test to see if parskip is larger than space between lines of % table. If not, do nothing. % If so, set to same dimension as multitablelinespace. \ifdim\multitableparskip>\multitablelinespace \global\multitableparskip=\multitablelinespace \global\advance\multitableparskip-7pt % to keep parskip somewhat smaller % than skip between lines in the table. \fi% \ifdim\multitableparskip=0pt \global\multitableparskip=\multitablelinespace \global\advance\multitableparskip-7pt % to keep parskip somewhat smaller % than skip between lines in the table. \fi} \message{conditionals,} % @iftex, @ifnotdocbook, @ifnothtml, @ifnotinfo, @ifnotplaintext, % @ifnotxml always succeed. They currently do nothing; we don't % attempt to check whether the conditionals are properly nested. But we % have to remember that they are conditionals, so that @end doesn't % attempt to close an environment group. % \def\makecond#1{% \expandafter\let\csname #1\endcsname = \relax \expandafter\let\csname iscond.#1\endcsname = 1 } \makecond{iftex} \makecond{ifnotdocbook} \makecond{ifnothtml} \makecond{ifnotinfo} \makecond{ifnotplaintext} \makecond{ifnotxml} % Ignore @ignore, @ifhtml, @ifinfo, and the like. % \def\direntry{\doignore{direntry}} \def\documentdescription{\doignore{documentdescription}} \def\docbook{\doignore{docbook}} \def\html{\doignore{html}} \def\ifdocbook{\doignore{ifdocbook}} \def\ifhtml{\doignore{ifhtml}} \def\ifinfo{\doignore{ifinfo}} \def\ifnottex{\doignore{ifnottex}} \def\ifplaintext{\doignore{ifplaintext}} \def\ifxml{\doignore{ifxml}} \def\ignore{\doignore{ignore}} \def\menu{\doignore{menu}} \def\xml{\doignore{xml}} % Ignore text until a line `@end #1', keeping track of nested conditionals. % % A count to remember the depth of nesting. \newcount\doignorecount \def\doignore#1{\begingroup % Scan in ``verbatim'' mode: \obeylines \catcode`\@ = \other \catcode`\{ = \other \catcode`\} = \other % % Make sure that spaces turn into tokens that match what \doignoretext wants. \spaceisspace % % Count number of #1's that we've seen. \doignorecount = 0 % % Swallow text until we reach the matching `@end #1'. \dodoignore{#1}% } { \catcode`_=11 % We want to use \_STOP_ which cannot appear in texinfo source. \obeylines % % \gdef\dodoignore#1{% % #1 contains the command name as a string, e.g., `ifinfo'. % % Define a command to find the next `@end #1'. \long\def\doignoretext##1^^M@end #1{% \doignoretextyyy##1^^M@#1\_STOP_}% % % And this command to find another #1 command, at the beginning of a % line. (Otherwise, we would consider a line `@c @ifset', for % example, to count as an @ifset for nesting.) \long\def\doignoretextyyy##1^^M@#1##2\_STOP_{\doignoreyyy{##2}\_STOP_}% % % And now expand that command. \doignoretext ^^M% }% } \def\doignoreyyy#1{% \def\temp{#1}% \ifx\temp\empty % Nothing found. \let\next\doignoretextzzz \else % Found a nested condition, ... \advance\doignorecount by 1 \let\next\doignoretextyyy % ..., look for another. % If we're here, #1 ends with ^^M\ifinfo (for example). \fi \next #1% the token \_STOP_ is present just after this macro. } % We have to swallow the remaining "\_STOP_". % \def\doignoretextzzz#1{% \ifnum\doignorecount = 0 % We have just found the outermost @end. \let\next\enddoignore \else % Still inside a nested condition. \advance\doignorecount by -1 \let\next\doignoretext % Look for the next @end. \fi \next } % Finish off ignored text. { \obeylines% % Ignore anything after the last `@end #1'; this matters in verbatim % environments, where otherwise the newline after an ignored conditional % would result in a blank line in the output. \gdef\enddoignore#1^^M{\endgroup\ignorespaces}% } % @set VAR sets the variable VAR to an empty value. % @set VAR REST-OF-LINE sets VAR to the value REST-OF-LINE. % % Since we want to separate VAR from REST-OF-LINE (which might be % empty), we can't just use \parsearg; we have to insert a space of our % own to delimit the rest of the line, and then take it out again if we % didn't need it. % We rely on the fact that \parsearg sets \catcode`\ =10. % \parseargdef\set{\setyyy#1 \endsetyyy} \def\setyyy#1 #2\endsetyyy{% {% \makevalueexpandable \def\temp{#2}% \edef\next{\gdef\makecsname{SET#1}}% \ifx\temp\empty \next{}% \else \setzzz#2\endsetzzz \fi }% } % Remove the trailing space \setxxx inserted. \def\setzzz#1 \endsetzzz{\next{#1}} % @clear VAR clears (i.e., unsets) the variable VAR. % \parseargdef\clear{% {% \makevalueexpandable \global\expandafter\let\csname SET#1\endcsname=\relax }% } % @value{foo} gets the text saved in variable foo. \def\value{\begingroup\makevalueexpandable\valuexxx} \def\valuexxx#1{\expandablevalue{#1}\endgroup} { \catcode`\-=\active \catcode`\_=\active % \gdef\makevalueexpandable{% \let\value = \expandablevalue % We don't want these characters active, ... \catcode`\-=\other \catcode`\_=\other % ..., but we might end up with active ones in the argument if % we're called from @code, as @code{@value{foo-bar_}}, though. % So \let them to their normal equivalents. \let-\normaldash \let_\normalunderscore } } % We have this subroutine so that we can handle at least some @value's % properly in indexes (we call \makevalueexpandable in \indexdummies). % The command has to be fully expandable (if the variable is set), since % the result winds up in the index file. This means that if the % variable's value contains other Texinfo commands, it's almost certain % it will fail (although perhaps we could fix that with sufficient work % to do a one-level expansion on the result, instead of complete). % % Unfortunately, this has the consequence that when _ is in the *value* % of an @set, it does not print properly in the roman fonts (get the cmr % dot accent at position 126 instead). No fix comes to mind, and it's % been this way since 2003 or earlier, so just ignore it. % \def\expandablevalue#1{% \expandafter\ifx\csname SET#1\endcsname\relax {[No value for ``#1'']}% \message{Variable `#1', used in @value, is not set.}% \else \csname SET#1\endcsname \fi } % Like \expandablevalue, but completely expandable (the \message in the % definition above operates at the execution level of TeX). Used when % writing to auxiliary files, due to the expansion that \write does. % If flag is undefined, pass through an unexpanded @value command: maybe it % will be set by the time it is read back in. % % NB flag names containing - or _ may not work here. \def\dummyvalue#1{% \expandafter\ifx\csname SET#1\endcsname\relax \noexpand\value{#1}% \else \csname SET#1\endcsname \fi } % Used for @value's in index entries to form the sort key: expand the @value % if possible, otherwise sort late. \def\indexnofontsvalue#1{% \expandafter\ifx\csname SET#1\endcsname\relax ZZZZZZZ \else \csname SET#1\endcsname \fi } % @ifset VAR ... @end ifset reads the `...' iff VAR has been defined % with @set. % % To get the special treatment we need for `@end ifset,' we call % \makecond and then redefine. % \makecond{ifset} \def\ifset{\parsearg{\doifset{\let\next=\ifsetfail}}} \def\doifset#1#2{% {% \makevalueexpandable \let\next=\empty \expandafter\ifx\csname SET#2\endcsname\relax #1% If not set, redefine \next. \fi \expandafter }\next } \def\ifsetfail{\doignore{ifset}} % @ifclear VAR ... @end executes the `...' iff VAR has never been % defined with @set, or has been undefined with @clear. % % The `\else' inside the `\doifset' parameter is a trick to reuse the % above code: if the variable is not set, do nothing, if it is set, % then redefine \next to \ifclearfail. % \makecond{ifclear} \def\ifclear{\parsearg{\doifset{\else \let\next=\ifclearfail}}} \def\ifclearfail{\doignore{ifclear}} % @ifcommandisdefined CMD ... @end executes the `...' if CMD (written % without the @) is in fact defined. We can only feasibly check at the % TeX level, so something like `mathcode' is going to considered % defined even though it is not a Texinfo command. % \makecond{ifcommanddefined} \def\ifcommanddefined{\parsearg{\doifcmddefined{\let\next=\ifcmddefinedfail}}} % \def\doifcmddefined#1#2{{% \makevalueexpandable \let\next=\empty \expandafter\ifx\csname #2\endcsname\relax #1% If not defined, \let\next as above. \fi \expandafter }\next } \def\ifcmddefinedfail{\doignore{ifcommanddefined}} % @ifcommandnotdefined CMD ... handled similar to @ifclear above. \makecond{ifcommandnotdefined} \def\ifcommandnotdefined{% \parsearg{\doifcmddefined{\else \let\next=\ifcmdnotdefinedfail}}} \def\ifcmdnotdefinedfail{\doignore{ifcommandnotdefined}} % Set the `txicommandconditionals' variable, so documents have a way to % test if the @ifcommand...defined conditionals are available. \set txicommandconditionals % @dircategory CATEGORY -- specify a category of the dir file % which this file should belong to. Ignore this in TeX. \let\dircategory=\comment % @defininfoenclose. \let\definfoenclose=\comment \message{indexing,} % Index generation facilities % Define \newwrite to be identical to plain tex's \newwrite % except not \outer, so it can be used within macros and \if's. \edef\newwrite{\makecsname{ptexnewwrite}} % \newindex {foo} defines an index named IX. % It automatically defines \IXindex such that % \IXindex ...rest of line... puts an entry in the index IX. % It also defines \IXindfile to be the number of the output channel for % the file that accumulates this index. The file's extension is IX. % The name of an index should be no more than 2 characters long % for the sake of vms. % \def\newindex#1{% \expandafter\chardef\csname#1indfile\endcsname=0 \expandafter\xdef\csname#1index\endcsname{% % Define @#1index \noexpand\doindex{#1}} } % @defindex foo == \newindex{foo} % \def\defindex{\parsearg\newindex} % Define @defcodeindex, like @defindex except put all entries in @code. % \def\defcodeindex{\parsearg\newcodeindex} % \def\newcodeindex#1{% \expandafter\chardef\csname#1indfile\endcsname=0 \expandafter\xdef\csname#1index\endcsname{% \noexpand\docodeindex{#1}}% } % The default indices: \newindex{cp}% concepts, \newcodeindex{fn}% functions, \newcodeindex{vr}% variables, \newcodeindex{tp}% types, \newcodeindex{ky}% keys \newcodeindex{pg}% and programs. % @synindex foo bar makes index foo feed into index bar. % Do this instead of @defindex foo if you don't want it as a separate index. % % @syncodeindex foo bar similar, but put all entries made for index foo % inside @code. % \def\synindex#1 #2 {\dosynindex\doindex{#1}{#2}} \def\syncodeindex#1 #2 {\dosynindex\docodeindex{#1}{#2}} % #1 is \doindex or \docodeindex, #2 the index getting redefined (foo), % #3 the target index (bar). \def\dosynindex#1#2#3{% \requireopenindexfile{#3}% % redefine \fooindfile: \expandafter\let\expandafter\temp\expandafter=\csname#3indfile\endcsname \expandafter\let\csname#2indfile\endcsname=\temp % redefine \fooindex: \expandafter\xdef\csname#2index\endcsname{\noexpand#1{#3}}% } % Define \doindex, the driver for all index macros. % Argument #1 is generated by the calling \fooindex macro, % and it is the two-letter name of the index. \def\doindex#1{\edef\indexname{#1}\parsearg\doindexxxx} \def\doindexxxx #1{\doind{\indexname}{#1}} % like the previous two, but they put @code around the argument. \def\docodeindex#1{\edef\indexname{#1}\parsearg\docodeindexxxx} \def\docodeindexxxx #1{\doind{\indexname}{\code{#1}}} % Used when writing an index entry out to an index file to prevent % expansion of Texinfo commands that can appear in an index entry. % \def\indexdummies{% \escapechar = `\\ % use backslash in output files. \definedummyletter\@% \definedummyletter\ % % % For texindex which always views { and } as separators. \def\{{\lbracechar{}}% \def\}{\rbracechar{}}% % % Do the redefinitions. \definedummies } % Used for the aux and toc files, where @ is the escape character. % \def\atdummies{% \definedummyletter\@% \definedummyletter\ % \definedummyletter\{% \definedummyletter\}% % % Do the redefinitions. \definedummies \otherbackslash } % \definedummyword defines \#1 as \string\#1\space, thus effectively % preventing its expansion. This is used only for control words, % not control letters, because the \space would be incorrect for % control characters, but is needed to separate the control word % from whatever follows. % % These can be used both for control words that take an argument and % those that do not. If it is followed by {arg} in the input, then % that will dutifully get written to the index (or wherever). % % For control letters, we have \definedummyletter, which omits the % space. % \def\definedummyword #1{\def#1{\string#1\space}}% \def\definedummyletter#1{\def#1{\string#1}}% \let\definedummyaccent\definedummyletter % Called from \indexdummies and \atdummies, to effectively prevent % the expansion of commands. % \def\definedummies{% % \let\commondummyword\definedummyword \let\commondummyletter\definedummyletter \let\commondummyaccent\definedummyaccent \commondummiesnofonts % \definedummyletter\_% \definedummyletter\-% % % Non-English letters. \definedummyword\AA \definedummyword\AE \definedummyword\DH \definedummyword\L \definedummyword\O \definedummyword\OE \definedummyword\TH \definedummyword\aa \definedummyword\ae \definedummyword\dh \definedummyword\exclamdown \definedummyword\l \definedummyword\o \definedummyword\oe \definedummyword\ordf \definedummyword\ordm \definedummyword\questiondown \definedummyword\ss \definedummyword\th % % Although these internal commands shouldn't show up, sometimes they do. \definedummyword\bf \definedummyword\gtr \definedummyword\hat \definedummyword\less \definedummyword\sf \definedummyword\sl \definedummyword\tclose \definedummyword\tt % \definedummyword\LaTeX \definedummyword\TeX % % Assorted special characters. \definedummyword\atchar \definedummyword\arrow \definedummyword\bullet \definedummyword\comma \definedummyword\copyright \definedummyword\registeredsymbol \definedummyword\dots \definedummyword\enddots \definedummyword\entrybreak \definedummyword\equiv \definedummyword\error \definedummyword\euro \definedummyword\expansion \definedummyword\geq \definedummyword\guillemetleft \definedummyword\guillemetright \definedummyword\guilsinglleft \definedummyword\guilsinglright \definedummyword\lbracechar \definedummyword\leq \definedummyword\mathopsup \definedummyword\minus \definedummyword\ogonek \definedummyword\pounds \definedummyword\point \definedummyword\print \definedummyword\quotedblbase \definedummyword\quotedblleft \definedummyword\quotedblright \definedummyword\quoteleft \definedummyword\quoteright \definedummyword\quotesinglbase \definedummyword\rbracechar \definedummyword\result \definedummyword\sub \definedummyword\sup \definedummyword\textdegree % % We want to disable all macros so that they are not expanded by \write. \macrolist \let\value\dummyvalue % \normalturnoffactive } % \commondummiesnofonts: common to \definedummies and \indexnofonts. % Define \commondummyletter, \commondummyaccent and \commondummyword before % using. Used for accents, font commands, and various control letters. % \def\commondummiesnofonts{% % Control letters and accents. \commondummyletter\!% \commondummyaccent\"% \commondummyaccent\'% \commondummyletter\*% \commondummyaccent\,% \commondummyletter\.% \commondummyletter\/% \commondummyletter\:% \commondummyaccent\=% \commondummyletter\?% \commondummyaccent\^% \commondummyaccent\`% \commondummyaccent\~% \commondummyword\u \commondummyword\v \commondummyword\H \commondummyword\dotaccent \commondummyword\ogonek \commondummyword\ringaccent \commondummyword\tieaccent \commondummyword\ubaraccent \commondummyword\udotaccent \commondummyword\dotless % % Texinfo font commands. \commondummyword\b \commondummyword\i \commondummyword\r \commondummyword\sansserif \commondummyword\sc \commondummyword\slanted \commondummyword\t % % Commands that take arguments. \commondummyword\abbr \commondummyword\acronym \commondummyword\anchor \commondummyword\cite \commondummyword\code \commondummyword\command \commondummyword\dfn \commondummyword\dmn \commondummyword\email \commondummyword\emph \commondummyword\env \commondummyword\file \commondummyword\image \commondummyword\indicateurl \commondummyword\inforef \commondummyword\kbd \commondummyword\key \commondummyword\math \commondummyword\option \commondummyword\pxref \commondummyword\ref \commondummyword\samp \commondummyword\strong \commondummyword\tie \commondummyword\U \commondummyword\uref \commondummyword\url \commondummyword\var \commondummyword\verb \commondummyword\w \commondummyword\xref } % For testing: output @{ and @} in index sort strings as \{ and \}. \newif\ifusebracesinindexes \let\indexlbrace\relax \let\indexrbrace\relax {\catcode`\@=0 \catcode`\\=13 @gdef@backslashdisappear{@def\{}} } { \catcode`\<=13 \catcode`\-=13 \catcode`\`=13 \gdef\indexnonalnumdisappear{% \expandafter\ifx\csname SETtxiindexlquoteignore\endcsname\relax\else % @set txiindexlquoteignore makes us ignore left quotes in the sort term. % (Introduced for FSFS 2nd ed.) \let`=\empty \fi % \expandafter\ifx\csname SETtxiindexbackslashignore\endcsname\relax\else \backslashdisappear \fi % \expandafter\ifx\csname SETtxiindexhyphenignore\endcsname\relax\else \def-{}% \fi \expandafter\ifx\csname SETtxiindexlessthanignore\endcsname\relax\else \def<{}% \fi \expandafter\ifx\csname SETtxiindexatsignignore\endcsname\relax\else \def\@{}% \fi } \gdef\indexnonalnumreappear{% \useindexbackslash \let-\normaldash \let<\normalless \def\@{@}% } } % \indexnofonts is used when outputting the strings to sort the index % by, and when constructing control sequence names. It eliminates all % control sequences and just writes whatever the best ASCII sort string % would be for a given command (usually its argument). % \def\indexnofonts{% % Accent commands should become @asis. \def\commondummyaccent##1{\let##1\asis}% % We can just ignore other control letters. \def\commondummyletter##1{\let##1\empty}% % All control words become @asis by default; overrides below. \let\commondummyword\commondummyaccent \commondummiesnofonts % % Don't no-op \tt, since it isn't a user-level command % and is used in the definitions of the active chars like <, >, |, etc. % Likewise with the other plain tex font commands. %\let\tt=\asis % \def\ { }% \def\@{@}% \def\_{\normalunderscore}% \def\-{}% @- shouldn't affect sorting % \uccode`\1=`\{ \uppercase{\def\{{1}}% \uccode`\1=`\} \uppercase{\def\}{1}}% \let\lbracechar\{% \let\rbracechar\}% % % Non-English letters. \def\AA{AA}% \def\AE{AE}% \def\DH{DZZ}% \def\L{L}% \def\OE{OE}% \def\O{O}% \def\TH{TH}% \def\aa{aa}% \def\ae{ae}% \def\dh{dzz}% \def\exclamdown{!}% \def\l{l}% \def\oe{oe}% \def\ordf{a}% \def\ordm{o}% \def\o{o}% \def\questiondown{?}% \def\ss{ss}% \def\th{th}% % \def\LaTeX{LaTeX}% \def\TeX{TeX}% % % Assorted special characters. \defglyph gives the control sequence a % definition that removes the {} that follows its use. \defglyph\atchar{@}% \defglyph\arrow{->}% \defglyph\bullet{bullet}% \defglyph\comma{,}% \defglyph\copyright{copyright}% \defglyph\dots{...}% \defglyph\enddots{...}% \defglyph\equiv{==}% \defglyph\error{error}% \defglyph\euro{euro}% \defglyph\expansion{==>}% \defglyph\geq{>=}% \defglyph\guillemetleft{<<}% \defglyph\guillemetright{>>}% \defglyph\guilsinglleft{<}% \defglyph\guilsinglright{>}% \defglyph\leq{<=}% \defglyph\lbracechar{\{}% \defglyph\minus{-}% \defglyph\point{.}% \defglyph\pounds{pounds}% \defglyph\print{-|}% \defglyph\quotedblbase{"}% \defglyph\quotedblleft{"}% \defglyph\quotedblright{"}% \defglyph\quoteleft{`}% \defglyph\quoteright{'}% \defglyph\quotesinglbase{,}% \defglyph\rbracechar{\}}% \defglyph\registeredsymbol{R}% \defglyph\result{=>}% \defglyph\textdegree{o}% % % We need to get rid of all macros, leaving only the arguments (if present). % Of course this is not nearly correct, but it is the best we can do for now. % makeinfo does not expand macros in the argument to @deffn, which ends up % writing an index entry, and texindex isn't prepared for an index sort entry % that starts with \. % % Since macro invocations are followed by braces, we can just redefine them % to take a single TeX argument. The case of a macro invocation that % goes to end-of-line is not handled. % \macrolist \let\value\indexnofontsvalue } \def\defglyph#1#2{\def#1##1{#2}} % see above \let\SETmarginindex=\relax % put index entries in margin (undocumented)? % Most index entries go through here, but \dosubind is the general case. % #1 is the index name, #2 is the entry text. \def\doind#1#2{\dosubind{#1}{#2}{}} % There is also \dosubind {index}{topic}{subtopic} % which makes an entry in a two-level index such as the operation index. % TODO: Two-level index? Operation index? % Workhorse for all indexes. % #1 is name of index, #2 is stuff to put there, #3 is subentry -- % empty if called from \doind, as we usually are (the main exception % is with most defuns, which call us directly). % \def\dosubind#1#2#3{% \iflinks {% \requireopenindexfile{#1}% % Store the main index entry text (including the third arg). \toks0 = {#2}% % If third arg is present, precede it with a space. \def\thirdarg{#3}% \ifx\thirdarg\empty \else \toks0 = \expandafter{\the\toks0 \space #3}% \fi % \edef\writeto{\csname#1indfile\endcsname}% % \safewhatsit\dosubindwrite }% \fi } % Check if an index file has been opened, and if not, open it. \def\requireopenindexfile#1{% \ifnum\csname #1indfile\endcsname=0 \expandafter\newwrite \csname#1indfile\endcsname \edef\suffix{#1}% % A .fls suffix would conflict with the file extension for the output % of -recorder, so use .f1s instead. \ifx\suffix\indexisfl\def\suffix{f1}\fi % Open the file \immediate\openout\csname#1indfile\endcsname \jobname.\suffix % Using \immediate above here prevents an object entering into the current % box, which could confound checks such as those in \safewhatsit for % preceding skips. \typeout{Writing index file \jobname.\suffix}% \fi} \def\indexisfl{fl} % Output \ as {\indexbackslash}, because \ is an escape character in % the index files. \let\indexbackslash=\relax {\catcode`\@=0 \catcode`\\=\active @gdef@useindexbackslash{@def\{{@indexbackslash}}} } % Definition for writing index entry text. \def\sortas#1{\ignorespaces}% % Definition for writing index entry sort key. Should occur at the at % the beginning of the index entry, like % @cindex @sortas{september} \september % The \ignorespaces takes care of following space, but there's no way % to remove space before it. { \catcode`\-=13 \gdef\indexwritesortas{% \begingroup \indexnonalnumreappear \indexwritesortasxxx} \gdef\indexwritesortasxxx#1{% \xdef\indexsortkey{#1}\endgroup} } % Write the entry in \toks0 to the index file. % \def\dosubindwrite{% % Put the index entry in the margin if desired. \ifx\SETmarginindex\relax\else \insert\margin{\hbox{\vrule height8pt depth3pt width0pt \the\toks0}}% \fi % % Remember, we are within a group. \indexdummies % Must do this here, since \bf, etc expand at this stage \useindexbackslash % \indexbackslash isn't defined now so it will be output % as is; and it will print as backslash. % The braces around \indexbrace are recognized by texindex. % % Get the string to sort by, by processing the index entry with all % font commands turned off. {\indexnofonts \def\lbracechar{{\indexlbrace}}% \def\rbracechar{{\indexrbrace}}% \let\{=\lbracechar \let\}=\rbracechar \indexnonalnumdisappear \xdef\indexsortkey{}% \let\sortas=\indexwritesortas \edef\temp{\the\toks0}% \setbox\dummybox = \hbox{\temp}% Make sure to execute any \sortas \ifx\indexsortkey\empty \xdef\indexsortkey{\temp}% \ifx\indexsortkey\empty\xdef\indexsortkey{ }\fi \fi }% % % Set up the complete index entry, with both the sort key and % the original text, including any font commands. We write % three arguments to \entry to the .?? file (four in the % subentry case), texindex reduces to two when writing the .??s % sorted result. \edef\temp{% \write\writeto{% \string\entry{\indexsortkey}{\noexpand\folio}{\the\toks0}}% }% \temp } \newbox\dummybox % used above % Take care of unwanted page breaks/skips around a whatsit: % % If a skip is the last thing on the list now, preserve it % by backing up by \lastskip, doing the \write, then inserting % the skip again. Otherwise, the whatsit generated by the % \write or \pdfdest will make \lastskip zero. The result is that % sequences like this: % @end defun % @tindex whatever % @defun ... % will have extra space inserted, because the \medbreak in the % start of the @defun won't see the skip inserted by the @end of % the previous defun. % % But don't do any of this if we're not in vertical mode. We % don't want to do a \vskip and prematurely end a paragraph. % % Avoid page breaks due to these extra skips, too. % % But wait, there is a catch there: % We'll have to check whether \lastskip is zero skip. \ifdim is not % sufficient for this purpose, as it ignores stretch and shrink parts % of the skip. The only way seems to be to check the textual % representation of the skip. % % The following is almost like \def\zeroskipmacro{0.0pt} except that % the ``p'' and ``t'' characters have catcode \other, not 11 (letter). % \edef\zeroskipmacro{\expandafter\the\csname z@skip\endcsname} % \newskip\whatsitskip \newcount\whatsitpenalty % % ..., ready, GO: % \def\safewhatsit#1{\ifhmode #1% \else % \lastskip and \lastpenalty cannot both be nonzero simultaneously. \whatsitskip = \lastskip \edef\lastskipmacro{\the\lastskip}% \whatsitpenalty = \lastpenalty % % If \lastskip is nonzero, that means the last item was a % skip. And since a skip is discardable, that means this % -\whatsitskip glue we're inserting is preceded by a % non-discardable item, therefore it is not a potential % breakpoint, therefore no \nobreak needed. \ifx\lastskipmacro\zeroskipmacro \else \vskip-\whatsitskip \fi % #1% % \ifx\lastskipmacro\zeroskipmacro % If \lastskip was zero, perhaps the last item was a penalty, and % perhaps it was >=10000, e.g., a \nobreak. In that case, we want % to re-insert the same penalty (values >10000 are used for various % signals); since we just inserted a non-discardable item, any % following glue (such as a \parskip) would be a breakpoint. For example: % @deffn deffn-whatever % @vindex index-whatever % Description. % would allow a break between the index-whatever whatsit % and the "Description." paragraph. \ifnum\whatsitpenalty>9999 \penalty\whatsitpenalty \fi \else % On the other hand, if we had a nonzero \lastskip, % this make-up glue would be preceded by a non-discardable item % (the whatsit from the \write), so we must insert a \nobreak. \nobreak\vskip\whatsitskip \fi \fi} % The index entry written in the file actually looks like % \entry {sortstring}{page}{topic} % or % \entry {sortstring}{page}{topic}{subtopic} % The texindex program reads in these files and writes files % containing these kinds of lines: % \initial {c} % before the first topic whose initial is c % \entry {topic}{pagelist} % for a topic that is used without subtopics % \primary {topic} % for the beginning of a topic that is used with subtopics % \secondary {subtopic}{pagelist} % for each subtopic. % Define the user-accessible indexing commands % @findex, @vindex, @kindex, @cindex. \def\findex {\fnindex} \def\kindex {\kyindex} \def\cindex {\cpindex} \def\vindex {\vrindex} \def\tindex {\tpindex} \def\pindex {\pgindex} \def\cindexsub {\begingroup\obeylines\cindexsub} {\obeylines % \gdef\cindexsub "#1" #2^^M{\endgroup % \dosubind{cp}{#2}{#1}}} % Define the macros used in formatting output of the sorted index material. % @printindex causes a particular index (the ??s file) to get printed. % It does not print any chapter heading (usually an @unnumbered). % \parseargdef\printindex{\begingroup \dobreak \chapheadingskip{10000}% % \smallfonts \rm \tolerance = 9500 \plainfrenchspacing \everypar = {}% don't want the \kern\-parindent from indentation suppression. % % See if the index file exists and is nonempty. % Change catcode of @ here so that if the index file contains % \initial {@} % as its first line, TeX doesn't complain about mismatched braces % (because it thinks @} is a control sequence). \catcode`\@ = 12 % See comment in \requireopenindexfile. \def\indexname{#1}\ifx\indexname\indexisfl\def\indexname{f1}\fi \openin 1 \jobname.\indexname s \ifeof 1 % \enddoublecolumns gets confused if there is no text in the index, % and it loses the chapter title and the aux file entries for the % index. The easiest way to prevent this problem is to make sure % there is some text. \putwordIndexNonexistent \typeout{No file \jobname.\indexname s.}% \else \catcode`\\ = 0 % % If the index file exists but is empty, then \openin leaves \ifeof % false. We have to make TeX try to read something from the file, so % it can discover if there is anything in it. \read 1 to \thisline \ifeof 1 \putwordIndexIsEmpty \else % Index files are almost Texinfo source, but we use \ as the escape % character. It would be better to use @, but that's too big a change % to make right now. \def\indexbackslash{\ttbackslash}% \let\indexlbrace\{ % Likewise, set these sequences for braces \let\indexrbrace\} % used in the sort key. \begindoublecolumns \let\dotheinsertentrybox\dotheinsertentryboxwithpenalty % % Read input from the index file line by line. \loopdo \ifeof1 \else \read 1 to \nextline \fi % \indexinputprocessing \thisline % \ifeof1\else \let\thisline\nextline \repeat %% \enddoublecolumns \fi \fi \closein 1 \endgroup} \def\loopdo#1\repeat{\def\body{#1}\loopdoxxx} \def\loopdoxxx{\let\next=\relax\body\let\next=\loopdoxxx\fi\next} \def\indexinputprocessing{% \ifeof1 \let\firsttoken\relax \else \edef\act{\gdef\noexpand\firsttoken{\getfirsttoken\nextline}}% \act \fi } \def\getfirsttoken#1{\expandafter\getfirsttokenx#1\endfirsttoken} \long\def\getfirsttokenx#1#2\endfirsttoken{\noexpand#1} % These macros are used by the sorted index file itself. % Change them to control the appearance of the index. {\catcode`\/=13 \catcode`\-=13 \catcode`\^=13 \catcode`\~=13 \catcode`\_=13 \catcode`\|=13 \catcode`\<=13 \catcode`\>=13 \catcode`\+=13 \catcode`\"=13 \catcode`\$=3 \gdef\initialglyphs{% % Some changes for non-alphabetic characters. Using the glyphs from the % math fonts looks more consistent than the typewriter font used elsewhere % for these characters. \def\indexbackslash{\math{\backslash}}% \let\\=\indexbackslash % % Can't get bold backslash so don't use bold forward slash \catcode`\/=13 \def/{{\secrmnotbold \normalslash}}% \def-{{\normaldash\normaldash}}% en dash `--' \def^{{\chapbf \normalcaret}}% \def~{{\chapbf \normaltilde}}% \def\_{% \leavevmode \kern.07em \vbox{\hrule width.3em height.1ex}\kern .07em }% \def|{$\vert$}% \def<{$\less$}% \def>{$\gtr$}% \def+{$\normalplus$}% }} \def\initial{% \bgroup \initialglyphs \initialx } \def\initialx#1{% % Remove any glue we may have, we'll be inserting our own. \removelastskip % % We like breaks before the index initials, so insert a bonus. % The glue before the bonus allows a little bit of space at the % bottom of a column to reduce an increase in inter-line spacing. \nobreak \vskip 0pt plus 5\baselineskip \penalty -300 \vskip 0pt plus -5\baselineskip % % Typeset the initial. Making this add up to a whole number of % baselineskips increases the chance of the dots lining up from column % to column. It still won't often be perfect, because of the stretch % we need before each entry, but it's better. % % No shrink because it confuses \balancecolumns. \vskip 1.67\baselineskip plus 1\baselineskip \leftline{\secfonts \kern-0.05em \secbf #1}% % \secfonts is inside the argument of \leftline so that the change of % \baselineskip will not affect any glue inserted before the vbox that % \leftline creates. % Do our best not to break after the initial. \nobreak \vskip .33\baselineskip plus .1\baselineskip \egroup % \initialglyphs } \newdimen\entryrightmargin \entryrightmargin=0pt % \entry typesets a paragraph consisting of the text (#1), dot leaders, and % then page number (#2) flushed to the right margin. It is used for index % and table of contents entries. The paragraph is indented by \leftskip. % \def\entry{% \begingroup % % For pdfTeX and XeTeX. % The redefinition of \domark stops marks being added in \pdflink to % preserve coloured links across page boundaries. Otherwise the marks % would get in the way of \lastbox in \insertentrybox. \let\domark\relax % % Start a new paragraph if necessary, so our assignments below can't % affect previous text. \par % % No extra space above this paragraph. \parskip = 0in % % When reading the text of entry, convert explicit line breaks % from @* into spaces. The user might give these in long section % titles, for instance. \def\*{\unskip\space\ignorespaces}% \def\entrybreak{\hfil\break}% An undocumented command % % Swallow the left brace of the text (first parameter): \afterassignment\doentry \let\temp = } \def\entrybreak{\unskip\space\ignorespaces}% \def\doentry{% % Save the text of the entry \global\setbox\boxA=\hbox\bgroup \bgroup % Instead of the swallowed brace. \noindent \aftergroup\finishentry % And now comes the text of the entry. % Not absorbing as a macro argument reduces the chance of problems % with catcodes occurring. } {\catcode`\@=11 \gdef\finishentry#1{% \egroup % end box A \dimen@ = \wd\boxA % Length of text of entry \global\setbox\boxA=\hbox\bgroup\unhbox\boxA % #1 is the page number. % % Get the width of the page numbers, and only use % leaders if they are present. \global\setbox\boxB = \hbox{#1}% \ifdim\wd\boxB = 0pt \null\nobreak\hfill\ % \else % \null\nobreak\indexdotfill % Have leaders before the page number. % \ifpdf \pdfgettoks#1.% \hskip\skip\thinshrinkable\the\toksA \else \ifx\XeTeXrevision\thisisundefined \hskip\skip\thinshrinkable #1% \else \pdfgettoks#1.% \hskip\skip\thinshrinkable\the\toksA \fi \fi \fi \egroup % end \boxA \ifdim\wd\boxB = 0pt \global\setbox\entrybox=\vbox{\unhbox\boxA}% \else \global\setbox\entrybox=\vbox\bgroup % We want the text of the entries to be aligned to the left, and the % page numbers to be aligned to the right. % \parindent = 0pt \advance\leftskip by 0pt plus 1fil \advance\leftskip by 0pt plus -1fill \rightskip = 0pt plus -1fil \advance\rightskip by 0pt plus 1fill % Cause last line, which could consist of page numbers on their own % if the list of page numbers is long, to be aligned to the right. \parfillskip=0pt plus -1fill % \advance\rightskip by \entryrightmargin % Determine how far we can stretch into the margin. % This allows, e.g., "Appendix H GNU Free Documentation License" to % fit on one line in @letterpaper format. \ifdim\entryrightmargin>2.1em \dimen@i=2.1em \else \dimen@i=0em \fi \advance \parfillskip by 0pt minus 1\dimen@i % \dimen@ii = \hsize \advance\dimen@ii by -1\leftskip \advance\dimen@ii by -1\entryrightmargin \advance\dimen@ii by 1\dimen@i \ifdim\wd\boxA > \dimen@ii % If the entry doesn't fit in one line \ifdim\dimen@ > 0.8\dimen@ii % due to long index text % Try to split the text roughly evenly. \dimen@ will be the length of % the first line. \dimen@ = 0.7\dimen@ \dimen@ii = \hsize \ifnum\dimen@>\dimen@ii % If the entry is too long (for example, if it needs more than % two lines), use all the space in the first line. \dimen@ = \dimen@ii \fi \advance\leftskip by 0pt plus 1fill % ragged right \advance \dimen@ by 1\rightskip \parshape = 2 0pt \dimen@ 0em \dimen@ii % Ideally we'd add a finite glue at the end of the first line only, % instead of using \parshape with explicit line lengths, but TeX % doesn't seem to provide a way to do such a thing. % % Indent all lines but the first one. \advance\leftskip by 1em \advance\parindent by -1em \fi\fi \indent % start paragraph \unhbox\boxA % % Do not prefer a separate line ending with a hyphen to fewer lines. \finalhyphendemerits = 0 % % Word spacing - no stretch \spaceskip=\fontdimen2\font minus \fontdimen4\font % \linepenalty=1000 % Discourage line breaks. \hyphenpenalty=5000 % Discourage hyphenation. % \par % format the paragraph \egroup % The \vbox \fi \endgroup \dotheinsertentrybox }} \newskip\thinshrinkable \skip\thinshrinkable=.15em minus .15em \newbox\entrybox \def\insertentrybox{% \ourunvbox\entrybox } % default definition \let\dotheinsertentrybox\insertentrybox % Use \lastbox to take apart vbox box by box, and add each sub-box % to the current vertical list. \def\ourunvbox#1{% \bgroup % for local binding of \delayedbox % Remove the last box from box #1 \global\setbox#1=\vbox{% \unvbox#1% \unskip % remove any glue \unpenalty \global\setbox\interbox=\lastbox }% \setbox\delayedbox=\box\interbox \ifdim\ht#1=0pt\else \ourunvbox#1 % Repeat on what's left of the box \nobreak \fi \box\delayedbox \egroup } \newbox\delayedbox \newbox\interbox % Used from \printindex. \firsttoken should be the first token % after the \entry. If it's not another \entry, we are at the last % line of a group of index entries, so insert a penalty to discourage % widowed index entries. \def\dotheinsertentryboxwithpenalty{% \ifx\firsttoken\isentry \else \penalty 9000 \fi \insertentrybox } \def\isentry{\entry}% % Like plain.tex's \dotfill, except uses up at least 1 em. % The filll stretch here overpowers both the fil and fill stretch to push % the page number to the right. \def\indexdotfill{\cleaders \hbox{$\mathsurround=0pt \mkern1.5mu.\mkern1.5mu$}\hskip 1em plus 1filll} \def\primary #1{\line{#1\hfil}} \newskip\secondaryindent \secondaryindent=0.5cm \def\secondary#1#2{{% \parfillskip=0in \parskip=0in \hangindent=1in \hangafter=1 \noindent\hskip\secondaryindent\hbox{#1}\indexdotfill \ifpdf \pdfgettoks#2.\ \the\toksA % The page number ends the paragraph. \else \ifx\XeTeXrevision\thisisundefined #2 \else \pdfgettoks#2.\ \the\toksA % The page number ends the paragraph. \fi \fi \par }} % Define two-column mode, which we use to typeset indexes. % Adapted from the TeXbook, page 416, which is to say, % the manmac.tex format used to print the TeXbook itself. \catcode`\@=11 % private names \newbox\partialpage \newdimen\doublecolumnhsize % Use inside an output routine to save \topmark and \firstmark \def\savemarks{% \global\savedtopmark=\expandafter{\topmark }% \global\savedfirstmark=\expandafter{\firstmark }% } \newtoks\savedtopmark \newtoks\savedfirstmark % Set \topmark and \firstmark for next time \output runs. % Can't be run from withinside \output (because any material % added while an output routine is active, including % penalties, is saved for after it finishes). The page so far % should be empty, otherwise what's on it will be thrown away. \def\restoremarks{% \mark{\the\savedtopmark}% \bgroup\output = {% \setbox\dummybox=\box\PAGE }abc\eject\egroup % "abc" because output routine doesn't fire for a completely empty page. \mark{\the\savedfirstmark}% } \def\begindoublecolumns{\begingroup % ended by \enddoublecolumns % If not much space left on page, start a new page. \ifdim\pagetotal>0.8\vsize\vfill\eject\fi % % Grab any single-column material above us. \output = {% % % Here is a possibility not foreseen in manmac: if we accumulate a % whole lot of material, we might end up calling this \output % routine twice in a row (see the doublecol-lose test, which is % essentially a couple of indexes with @setchapternewpage off). In % that case we just ship out what is in \partialpage with the normal % output routine. Generally, \partialpage will be empty when this % runs and this will be a no-op. See the indexspread.tex test case. \ifvoid\partialpage \else \onepageout{\pagecontents\partialpage}% \fi % \global\setbox\partialpage = \vbox{% % Unvbox the main output page. \unvbox\PAGE \kern-\topskip \kern\baselineskip }% \savemarks }% \eject % run that output routine to set \partialpage \restoremarks % % We recover the two marks that the last output routine saved in order % to propagate the information in marks added around a chapter heading, % which could be otherwise be lost by the time the final page is output. % % % Use the double-column output routine for subsequent pages. \output = {\doublecolumnout}% % % Change the page size parameters. We could do this once outside this % routine, in each of @smallbook, @afourpaper, and the default 8.5x11 % format, but then we repeat the same computation. Repeating a couple % of assignments once per index is clearly meaningless for the % execution time, so we may as well do it in one place. % % First we halve the line length, less a little for the gutter between % the columns. We compute the gutter based on the line length, so it % changes automatically with the paper format. The magic constant % below is chosen so that the gutter has the same value (well, +-<1pt) % as it did when we hard-coded it. % % We put the result in a separate register, \doublecolumhsize, so we % can restore it in \pagesofar, after \hsize itself has (potentially) % been clobbered. % \doublecolumnhsize = \hsize \advance\doublecolumnhsize by -.04154\hsize \divide\doublecolumnhsize by 2 \hsize = \doublecolumnhsize % % Double the \vsize as well. \advance\vsize by -\ht\partialpage \vsize = 2\vsize % % For the benefit of balancing columns \advance\baselineskip by 0pt plus 0.5pt } % The double-column output routine for all double-column pages except % the last, which is done by \balancecolumns. % \def\doublecolumnout{% % \splittopskip=\topskip \splitmaxdepth=\maxdepth % Get the available space for the double columns -- the normal % (undoubled) page height minus any material left over from the % previous page. \dimen@ = \vsize \divide\dimen@ by 2 % % box0 will be the left-hand column, box2 the right. \setbox0=\vsplit\PAGE to\dimen@ \setbox2=\vsplit\PAGE to\dimen@ \global\advance\vsize by 2\ht\partialpage \onepageout\pagesofar \unvbox\PAGE \penalty\outputpenalty } % % Re-output the contents of the output page -- any previous material, % followed by the two boxes we just split, in box0 and box2. \def\pagesofar{% \unvbox\partialpage % \hsize = \doublecolumnhsize \wd0=\hsize \wd2=\hsize \hbox to\txipagewidth{\box0\hfil\box2}% } % Finished with with double columns. \def\enddoublecolumns{% % The following penalty ensures that the page builder is exercised % _before_ we change the output routine. This is necessary in the % following situation: % % The last section of the index consists only of a single entry. % Before this section, \pagetotal is less than \pagegoal, so no % break occurs before the last section starts. However, the last % section, consisting of \initial and the single \entry, does not % fit on the page and has to be broken off. Without the following % penalty the page builder will not be exercised until \eject % below, and by that time we'll already have changed the output % routine to the \balancecolumns version, so the next-to-last % double-column page will be processed with \balancecolumns, which % is wrong: The two columns will go to the main vertical list, with % the broken-off section in the recent contributions. As soon as % the output routine finishes, TeX starts reconsidering the page % break. The two columns and the broken-off section both fit on the % page, because the two columns now take up only half of the page % goal. When TeX sees \eject from below which follows the final % section, it invokes the new output routine that we've set after % \balancecolumns below; \onepageout will try to fit the two columns % and the final section into the vbox of \txipageheight (see % \pagebody), causing an overfull box. % % Note that glue won't work here, because glue does not exercise the % page builder, unlike penalties (see The TeXbook, pp. 280-281). \penalty0 % \output = {% % Split the last of the double-column material. \savemarks \balancecolumns }% \eject % call the \output just set \ifdim\pagetotal=0pt % Having called \balancecolumns once, we do not % want to call it again. Therefore, reset \output to its normal % definition right away. \global\output = {\onepageout{\pagecontents\PAGE}}% % \endgroup % started in \begindoublecolumns \restoremarks % Leave the double-column material on the current page, no automatic % page break. \box\balancedcolumns % % \pagegoal was set to the doubled \vsize above, since we restarted % the current page. We're now back to normal single-column % typesetting, so reset \pagegoal to the normal \vsize. \global\vsize = \txipageheight % \pagegoal = \txipageheight % \else % We had some left-over material. This might happen when \doublecolumnout % is called in \balancecolumns. Try again. \expandafter\enddoublecolumns \fi } \newbox\balancedcolumns \setbox\balancedcolumns=\vbox{shouldnt see this}% % % Only called for the last of the double column material. \doublecolumnout % does the others. \def\balancecolumns{% \setbox0 = \vbox{\unvbox\PAGE}% like \box255 but more efficient, see p.120. \dimen@ = \ht0 \advance\dimen@ by \topskip \advance\dimen@ by-\baselineskip \ifdim\dimen@<5\baselineskip % Don't split a short final column in two. \setbox2=\vbox{}% \global\setbox\balancedcolumns=\vbox{\pagesofar}% \else \divide\dimen@ by 2 % target to split to \dimen@ii = \dimen@ \splittopskip = \topskip % Loop until left column is at least as high as the right column. {% \vbadness = 10000 \loop \global\setbox3 = \copy0 \global\setbox1 = \vsplit3 to \dimen@ \ifdim\ht1<\ht3 \global\advance\dimen@ by 1pt \repeat }% % Now the left column is in box 1, and the right column in box 3. % % Check whether the left column has come out higher than the page itself. % (Note that we have doubled \vsize for the double columns, so % the actual height of the page is 0.5\vsize). \ifdim2\ht1>\vsize % It appears that we have been called upon to balance too much material. % Output some of it with \doublecolumnout, leaving the rest on the page. \setbox\PAGE=\box0 \doublecolumnout \else % Compare the heights of the two columns. \ifdim4\ht1>5\ht3 % Column heights are too different, so don't make their bottoms % flush with each other. \setbox2=\vbox to \ht1 {\unvbox3\vfill}% \setbox0=\vbox to \ht1 {\unvbox1\vfill}% \else % Make column bottoms flush with each other. \setbox2=\vbox to\ht1{\unvbox3\unskip}% \setbox0=\vbox to\ht1{\unvbox1\unskip}% \fi \global\setbox\balancedcolumns=\vbox{\pagesofar}% \fi \fi % } \catcode`\@ = \other \message{sectioning,} % Chapters, sections, etc. % Let's start with @part. \outer\parseargdef\part{\partzzz{#1}} \def\partzzz#1{% \chapoddpage \null \vskip.3\vsize % move it down on the page a bit \begingroup \noindent \titlefonts\rm #1\par % the text \let\lastnode=\empty % no node to associate with \writetocentry{part}{#1}{}% but put it in the toc \headingsoff % no headline or footline on the part page % This outputs a mark at the end of the page that clears \thischapter % and \thissection, as is done in \startcontents. \let\pchapsepmacro\relax \chapmacro{}{Yomitfromtoc}{}% \chapoddpage \endgroup } % \unnumberedno is an oxymoron. But we count the unnumbered % sections so that we can refer to them unambiguously in the pdf % outlines by their "section number". We avoid collisions with chapter % numbers by starting them at 10000. (If a document ever has 10000 % chapters, we're in trouble anyway, I'm sure.) \newcount\unnumberedno \unnumberedno = 10000 \newcount\chapno \newcount\secno \secno=0 \newcount\subsecno \subsecno=0 \newcount\subsubsecno \subsubsecno=0 % This counter is funny since it counts through charcodes of letters A, B, ... \newcount\appendixno \appendixno = `\@ % % \def\appendixletter{\char\the\appendixno} % We do the following ugly conditional instead of the above simple % construct for the sake of pdftex, which needs the actual % letter in the expansion, not just typeset. % \def\appendixletter{% \ifnum\appendixno=`A A% \else\ifnum\appendixno=`B B% \else\ifnum\appendixno=`C C% \else\ifnum\appendixno=`D D% \else\ifnum\appendixno=`E E% \else\ifnum\appendixno=`F F% \else\ifnum\appendixno=`G G% \else\ifnum\appendixno=`H H% \else\ifnum\appendixno=`I I% \else\ifnum\appendixno=`J J% \else\ifnum\appendixno=`K K% \else\ifnum\appendixno=`L L% \else\ifnum\appendixno=`M M% \else\ifnum\appendixno=`N N% \else\ifnum\appendixno=`O O% \else\ifnum\appendixno=`P P% \else\ifnum\appendixno=`Q Q% \else\ifnum\appendixno=`R R% \else\ifnum\appendixno=`S S% \else\ifnum\appendixno=`T T% \else\ifnum\appendixno=`U U% \else\ifnum\appendixno=`V V% \else\ifnum\appendixno=`W W% \else\ifnum\appendixno=`X X% \else\ifnum\appendixno=`Y Y% \else\ifnum\appendixno=`Z Z% % The \the is necessary, despite appearances, because \appendixletter is % expanded while writing the .toc file. \char\appendixno is not % expandable, thus it is written literally, thus all appendixes come out % with the same letter (or @) in the toc without it. \else\char\the\appendixno \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi \fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi\fi} % Each @chapter defines these (using marks) as the number+name, number % and name of the chapter. Page headings and footings can use % these. @section does likewise. \def\thischapter{} \def\thischapternum{} \def\thischaptername{} \def\thissection{} \def\thissectionnum{} \def\thissectionname{} \newcount\absseclevel % used to calculate proper heading level \newcount\secbase\secbase=0 % @raisesections/@lowersections modify this count % @raisesections: treat @section as chapter, @subsection as section, etc. \def\raisesections{\global\advance\secbase by -1} \let\up=\raisesections % original BFox name % @lowersections: treat @chapter as section, @section as subsection, etc. \def\lowersections{\global\advance\secbase by 1} \let\down=\lowersections % original BFox name % we only have subsub. \chardef\maxseclevel = 3 % % A numbered section within an unnumbered changes to unnumbered too. % To achieve this, remember the "biggest" unnum. sec. we are currently in: \chardef\unnlevel = \maxseclevel % % Trace whether the current chapter is an appendix or not: % \chapheadtype is "N" or "A", unnumbered chapters are ignored. \def\chapheadtype{N} % Choose a heading macro % #1 is heading type % #2 is heading level % #3 is text for heading \def\genhead#1#2#3{% % Compute the abs. sec. level: \absseclevel=#2 \advance\absseclevel by \secbase % Make sure \absseclevel doesn't fall outside the range: \ifnum \absseclevel < 0 \absseclevel = 0 \else \ifnum \absseclevel > 3 \absseclevel = 3 \fi \fi % The heading type: \def\headtype{#1}% \if \headtype U% \ifnum \absseclevel < \unnlevel \chardef\unnlevel = \absseclevel \fi \else % Check for appendix sections: \ifnum \absseclevel = 0 \edef\chapheadtype{\headtype}% \else \if \headtype A\if \chapheadtype N% \errmessage{@appendix... within a non-appendix chapter}% \fi\fi \fi % Check for numbered within unnumbered: \ifnum \absseclevel > \unnlevel \def\headtype{U}% \else \chardef\unnlevel = 3 \fi \fi % Now print the heading: \if \headtype U% \ifcase\absseclevel \unnumberedzzz{#3}% \or \unnumberedseczzz{#3}% \or \unnumberedsubseczzz{#3}% \or \unnumberedsubsubseczzz{#3}% \fi \else \if \headtype A% \ifcase\absseclevel \appendixzzz{#3}% \or \appendixsectionzzz{#3}% \or \appendixsubseczzz{#3}% \or \appendixsubsubseczzz{#3}% \fi \else \ifcase\absseclevel \chapterzzz{#3}% \or \seczzz{#3}% \or \numberedsubseczzz{#3}% \or \numberedsubsubseczzz{#3}% \fi \fi \fi \suppressfirstparagraphindent } % an interface: \def\numhead{\genhead N} \def\apphead{\genhead A} \def\unnmhead{\genhead U} % @chapter, @appendix, @unnumbered. Increment top-level counter, reset % all lower-level sectioning counters to zero. % % Also set \chaplevelprefix, which we prepend to @float sequence numbers % (e.g., figures), q.v. By default (before any chapter), that is empty. \let\chaplevelprefix = \empty % \outer\parseargdef\chapter{\numhead0{#1}} % normally numhead0 calls chapterzzz \def\chapterzzz#1{% % section resetting is \global in case the chapter is in a group, such % as an @include file. \global\secno=0 \global\subsecno=0 \global\subsubsecno=0 \global\advance\chapno by 1 % % Used for \float. \gdef\chaplevelprefix{\the\chapno.}% \resetallfloatnos % % \putwordChapter can contain complex things in translations. \toks0=\expandafter{\putwordChapter}% \message{\the\toks0 \space \the\chapno}% % % Write the actual heading. \chapmacro{#1}{Ynumbered}{\the\chapno}% % % So @section and the like are numbered underneath this chapter. \global\let\section = \numberedsec \global\let\subsection = \numberedsubsec \global\let\subsubsection = \numberedsubsubsec } \outer\parseargdef\appendix{\apphead0{#1}} % normally calls appendixzzz % \def\appendixzzz#1{% \global\secno=0 \global\subsecno=0 \global\subsubsecno=0 \global\advance\appendixno by 1 \gdef\chaplevelprefix{\appendixletter.}% \resetallfloatnos % % \putwordAppendix can contain complex things in translations. \toks0=\expandafter{\putwordAppendix}% \message{\the\toks0 \space \appendixletter}% % \chapmacro{#1}{Yappendix}{\appendixletter}% % \global\let\section = \appendixsec \global\let\subsection = \appendixsubsec \global\let\subsubsection = \appendixsubsubsec } % normally unnmhead0 calls unnumberedzzz: \outer\parseargdef\unnumbered{\unnmhead0{#1}} \def\unnumberedzzz#1{% \global\secno=0 \global\subsecno=0 \global\subsubsecno=0 \global\advance\unnumberedno by 1 % % Since an unnumbered has no number, no prefix for figures. \global\let\chaplevelprefix = \empty \resetallfloatnos % % This used to be simply \message{#1}, but TeX fully expands the % argument to \message. Therefore, if #1 contained @-commands, TeX % expanded them. For example, in `@unnumbered The @cite{Book}', TeX % expanded @cite (which turns out to cause errors because \cite is meant % to be executed, not expanded). % % Anyway, we don't want the fully-expanded definition of @cite to appear % as a result of the \message, we just want `@cite' itself. We use % \the<toks register> to achieve this: TeX expands \the<toks> only once, % simply yielding the contents of <toks register>. (We also do this for % the toc entries.) \toks0 = {#1}% \message{(\the\toks0)}% % \chapmacro{#1}{Ynothing}{\the\unnumberedno}% % \global\let\section = \unnumberedsec \global\let\subsection = \unnumberedsubsec \global\let\subsubsection = \unnumberedsubsubsec } % @centerchap is like @unnumbered, but the heading is centered. \outer\parseargdef\centerchap{% \let\centerparametersmaybe = \centerparameters \unnmhead0{#1}% \let\centerparametersmaybe = \relax } % @top is like @unnumbered. \let\top\unnumbered % Sections. % \outer\parseargdef\numberedsec{\numhead1{#1}} % normally calls seczzz \def\seczzz#1{% \global\subsecno=0 \global\subsubsecno=0 \global\advance\secno by 1 \sectionheading{#1}{sec}{Ynumbered}{\the\chapno.\the\secno}% } % normally calls appendixsectionzzz: \outer\parseargdef\appendixsection{\apphead1{#1}} \def\appendixsectionzzz#1{% \global\subsecno=0 \global\subsubsecno=0 \global\advance\secno by 1 \sectionheading{#1}{sec}{Yappendix}{\appendixletter.\the\secno}% } \let\appendixsec\appendixsection % normally calls unnumberedseczzz: \outer\parseargdef\unnumberedsec{\unnmhead1{#1}} \def\unnumberedseczzz#1{% \global\subsecno=0 \global\subsubsecno=0 \global\advance\secno by 1 \sectionheading{#1}{sec}{Ynothing}{\the\unnumberedno.\the\secno}% } % Subsections. % % normally calls numberedsubseczzz: \outer\parseargdef\numberedsubsec{\numhead2{#1}} \def\numberedsubseczzz#1{% \global\subsubsecno=0 \global\advance\subsecno by 1 \sectionheading{#1}{subsec}{Ynumbered}{\the\chapno.\the\secno.\the\subsecno}% } % normally calls appendixsubseczzz: \outer\parseargdef\appendixsubsec{\apphead2{#1}} \def\appendixsubseczzz#1{% \global\subsubsecno=0 \global\advance\subsecno by 1 \sectionheading{#1}{subsec}{Yappendix}% {\appendixletter.\the\secno.\the\subsecno}% } % normally calls unnumberedsubseczzz: \outer\parseargdef\unnumberedsubsec{\unnmhead2{#1}} \def\unnumberedsubseczzz#1{% \global\subsubsecno=0 \global\advance\subsecno by 1 \sectionheading{#1}{subsec}{Ynothing}% {\the\unnumberedno.\the\secno.\the\subsecno}% } % Subsubsections. % % normally numberedsubsubseczzz: \outer\parseargdef\numberedsubsubsec{\numhead3{#1}} \def\numberedsubsubseczzz#1{% \global\advance\subsubsecno by 1 \sectionheading{#1}{subsubsec}{Ynumbered}% {\the\chapno.\the\secno.\the\subsecno.\the\subsubsecno}% } % normally appendixsubsubseczzz: \outer\parseargdef\appendixsubsubsec{\apphead3{#1}} \def\appendixsubsubseczzz#1{% \global\advance\subsubsecno by 1 \sectionheading{#1}{subsubsec}{Yappendix}% {\appendixletter.\the\secno.\the\subsecno.\the\subsubsecno}% } % normally unnumberedsubsubseczzz: \outer\parseargdef\unnumberedsubsubsec{\unnmhead3{#1}} \def\unnumberedsubsubseczzz#1{% \global\advance\subsubsecno by 1 \sectionheading{#1}{subsubsec}{Ynothing}% {\the\unnumberedno.\the\secno.\the\subsecno.\the\subsubsecno}% } % These macros control what the section commands do, according % to what kind of chapter we are in (ordinary, appendix, or unnumbered). % Define them by default for a numbered chapter. \let\section = \numberedsec \let\subsection = \numberedsubsec \let\subsubsection = \numberedsubsubsec % Define @majorheading, @heading and @subheading \def\majorheading{% {\advance\chapheadingskip by 10pt \chapbreak }% \parsearg\chapheadingzzz } \def\chapheading{\chapbreak \parsearg\chapheadingzzz} \def\chapheadingzzz#1{% \vbox{\chapfonts \raggedtitlesettings #1\par}% \nobreak\bigskip \nobreak \suppressfirstparagraphindent } % @heading, @subheading, @subsubheading. \parseargdef\heading{\sectionheading{#1}{sec}{Yomitfromtoc}{} \suppressfirstparagraphindent} \parseargdef\subheading{\sectionheading{#1}{subsec}{Yomitfromtoc}{} \suppressfirstparagraphindent} \parseargdef\subsubheading{\sectionheading{#1}{subsubsec}{Yomitfromtoc}{} \suppressfirstparagraphindent} % These macros generate a chapter, section, etc. heading only % (including whitespace, linebreaking, etc. around it), % given all the information in convenient, parsed form. % Args are the skip and penalty (usually negative) \def\dobreak#1#2{\par\ifdim\lastskip<#1\removelastskip\penalty#2\vskip#1\fi} % Parameter controlling skip before chapter headings (if needed) \newskip\chapheadingskip % Define plain chapter starts, and page on/off switching for it. \def\chapbreak{\dobreak \chapheadingskip {-4000}} % Start a new page \def\chappager{\par\vfill\supereject} % \chapoddpage - start on an odd page for a new chapter % Because \domark is called before \chapoddpage, the filler page will % get the headings for the next chapter, which is wrong. But we don't % care -- we just disable all headings on the filler page. \def\chapoddpage{% \chappager \ifodd\pageno \else \begingroup \headingsoff \null \chappager \endgroup \fi } \parseargdef\setchapternewpage{\csname CHAPPAG#1\endcsname} \def\CHAPPAGoff{% \global\let\contentsalignmacro = \chappager \global\let\pchapsepmacro=\chapbreak \global\let\pagealignmacro=\chappager} \def\CHAPPAGon{% \global\let\contentsalignmacro = \chappager \global\let\pchapsepmacro=\chappager \global\let\pagealignmacro=\chappager \global\def\HEADINGSon{\HEADINGSsingle}} \def\CHAPPAGodd{% \global\let\contentsalignmacro = \chapoddpage \global\let\pchapsepmacro=\chapoddpage \global\let\pagealignmacro=\chapoddpage \global\def\HEADINGSon{\HEADINGSdouble}} \CHAPPAGon % \chapmacro - Chapter opening. % % #1 is the text, #2 is the section type (Ynumbered, Ynothing, % Yappendix, Yomitfromtoc), #3 the chapter number. % Not used for @heading series. % % To test against our argument. \def\Ynothingkeyword{Ynothing} \def\Yappendixkeyword{Yappendix} \def\Yomitfromtockeyword{Yomitfromtoc} % \def\chapmacro#1#2#3{% \expandafter\ifx\thisenv\titlepage\else \checkenv{}% chapters, etc., should not start inside an environment. \fi % FIXME: \chapmacro is currently called from inside \titlepage when % \setcontentsaftertitlepage to print the "Table of Contents" heading, but % this should probably be done by \sectionheading with an option to print % in chapter size. % % Insert the first mark before the heading break (see notes for \domark). \let\prevchapterdefs=\lastchapterdefs \let\prevsectiondefs=\lastsectiondefs \gdef\lastsectiondefs{\gdef\thissectionname{}\gdef\thissectionnum{}% \gdef\thissection{}}% % \def\temptype{#2}% \ifx\temptype\Ynothingkeyword \gdef\lastchapterdefs{\gdef\thischaptername{#1}\gdef\thischapternum{}% \gdef\thischapter{\thischaptername}}% \else\ifx\temptype\Yomitfromtockeyword \gdef\lastchapterdefs{\gdef\thischaptername{#1}\gdef\thischapternum{}% \gdef\thischapter{}}% \else\ifx\temptype\Yappendixkeyword \toks0={#1}% \xdef\lastchapterdefs{% \gdef\noexpand\thischaptername{\the\toks0}% \gdef\noexpand\thischapternum{\appendixletter}% % \noexpand\putwordAppendix avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thischapter{\noexpand\putwordAppendix{} \noexpand\thischapternum: \noexpand\thischaptername}% }% \else \toks0={#1}% \xdef\lastchapterdefs{% \gdef\noexpand\thischaptername{\the\toks0}% \gdef\noexpand\thischapternum{\the\chapno}% % \noexpand\putwordChapter avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thischapter{\noexpand\putwordChapter{} \noexpand\thischapternum: \noexpand\thischaptername}% }% \fi\fi\fi % % Output the mark. Pass it through \safewhatsit, to take care of % the preceding space. \safewhatsit\domark % % Insert the chapter heading break. \pchapsepmacro % % Now the second mark, after the heading break. No break points % between here and the heading. \let\prevchapterdefs=\lastchapterdefs \let\prevsectiondefs=\lastsectiondefs \domark % {% \chapfonts \rm \let\footnote=\errfootnoteheading % give better error message % % Have to define \lastsection before calling \donoderef, because the % xref code eventually uses it. On the other hand, it has to be called % after \pchapsepmacro, or the headline will change too soon. \gdef\lastsection{#1}% % % Only insert the separating space if we have a chapter/appendix % number, and don't print the unnumbered ``number''. \ifx\temptype\Ynothingkeyword \setbox0 = \hbox{}% \def\toctype{unnchap}% \else\ifx\temptype\Yomitfromtockeyword \setbox0 = \hbox{}% contents like unnumbered, but no toc entry \def\toctype{omit}% \else\ifx\temptype\Yappendixkeyword \setbox0 = \hbox{\putwordAppendix{} #3\enspace}% \def\toctype{app}% \else \setbox0 = \hbox{#3\enspace}% \def\toctype{numchap}% \fi\fi\fi % % Write the toc entry for this chapter. Must come before the % \donoderef, because we include the current node name in the toc % entry, and \donoderef resets it to empty. \writetocentry{\toctype}{#1}{#3}% % % For pdftex, we have to write out the node definition (aka, make % the pdfdest) after any page break, but before the actual text has % been typeset. If the destination for the pdf outline is after the % text, then jumping from the outline may wind up with the text not % being visible, for instance under high magnification. \donoderef{#2}% % % Typeset the actual heading. \nobreak % Avoid page breaks at the interline glue. \vbox{\raggedtitlesettings \hangindent=\wd0 \centerparametersmaybe \unhbox0 #1\par}% }% \nobreak\bigskip % no page break after a chapter title \nobreak } % @centerchap -- centered and unnumbered. \let\centerparametersmaybe = \relax \def\centerparameters{% \advance\rightskip by 3\rightskip \leftskip = \rightskip \parfillskip = 0pt } % Section titles. These macros combine the section number parts and % call the generic \sectionheading to do the printing. % \newskip\secheadingskip \def\secheadingbreak{\dobreak \secheadingskip{-1000}} % Subsection titles. \newskip\subsecheadingskip \def\subsecheadingbreak{\dobreak \subsecheadingskip{-500}} % Subsubsection titles. \def\subsubsecheadingskip{\subsecheadingskip} \def\subsubsecheadingbreak{\subsecheadingbreak} % Print any size, any type, section title. % % #1 is the text of the title, % #2 is the section level (sec/subsec/subsubsec), % #3 is the section type (Ynumbered, Ynothing, Yappendix, Yomitfromtoc), % #4 is the section number. % \def\seckeyword{sec} % \def\sectionheading#1#2#3#4{% {% \def\sectionlevel{#2}% \def\temptype{#3}% % % It is ok for the @heading series commands to appear inside an % environment (it's been historically allowed, though the logic is % dubious), but not the others. \ifx\temptype\Yomitfromtockeyword\else \checkenv{}% non-@*heading should not be in an environment. \fi \let\footnote=\errfootnoteheading % % Switch to the right set of fonts. \csname #2fonts\endcsname \rm % % Insert first mark before the heading break (see notes for \domark). \let\prevsectiondefs=\lastsectiondefs \ifx\temptype\Ynothingkeyword \ifx\sectionlevel\seckeyword \gdef\lastsectiondefs{\gdef\thissectionname{#1}\gdef\thissectionnum{}% \gdef\thissection{\thissectionname}}% \fi \else\ifx\temptype\Yomitfromtockeyword % Don't redefine \thissection. \else\ifx\temptype\Yappendixkeyword \ifx\sectionlevel\seckeyword \toks0={#1}% \xdef\lastsectiondefs{% \gdef\noexpand\thissectionname{\the\toks0}% \gdef\noexpand\thissectionnum{#4}% % \noexpand\putwordSection avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thissection{\noexpand\putwordSection{} \noexpand\thissectionnum: \noexpand\thissectionname}% }% \fi \else \ifx\sectionlevel\seckeyword \toks0={#1}% \xdef\lastsectiondefs{% \gdef\noexpand\thissectionname{\the\toks0}% \gdef\noexpand\thissectionnum{#4}% % \noexpand\putwordSection avoids expanding indigestible % commands in some of the translations. \gdef\noexpand\thissection{\noexpand\putwordSection{} \noexpand\thissectionnum: \noexpand\thissectionname}% }% \fi \fi\fi\fi % % Go into vertical mode. Usually we'll already be there, but we % don't want the following whatsit to end up in a preceding paragraph % if the document didn't happen to have a blank line. \par % % Output the mark. Pass it through \safewhatsit, to take care of % the preceding space. \safewhatsit\domark % % Insert space above the heading. \csname #2headingbreak\endcsname % % Now the second mark, after the heading break. No break points % between here and the heading. \global\let\prevsectiondefs=\lastsectiondefs \domark % % Only insert the space after the number if we have a section number. \ifx\temptype\Ynothingkeyword \setbox0 = \hbox{}% \def\toctype{unn}% \gdef\lastsection{#1}% \else\ifx\temptype\Yomitfromtockeyword % for @headings -- no section number, don't include in toc, % and don't redefine \lastsection. \setbox0 = \hbox{}% \def\toctype{omit}% \let\sectionlevel=\empty \else\ifx\temptype\Yappendixkeyword \setbox0 = \hbox{#4\enspace}% \def\toctype{app}% \gdef\lastsection{#1}% \else \setbox0 = \hbox{#4\enspace}% \def\toctype{num}% \gdef\lastsection{#1}% \fi\fi\fi % % Write the toc entry (before \donoderef). See comments in \chapmacro. \writetocentry{\toctype\sectionlevel}{#1}{#4}% % % Write the node reference (= pdf destination for pdftex). % Again, see comments in \chapmacro. \donoderef{#3}% % % Interline glue will be inserted when the vbox is completed. % That glue will be a valid breakpoint for the page, since it'll be % preceded by a whatsit (usually from the \donoderef, or from the % \writetocentry if there was no node). We don't want to allow that % break, since then the whatsits could end up on page n while the % section is on page n+1, thus toc/etc. are wrong. Debian bug 276000. \nobreak % % Output the actual section heading. \vbox{\hyphenpenalty=10000 \tolerance=5000 \parindent=0pt \ptexraggedright \hangindent=\wd0 % zero if no section number \unhbox0 #1}% }% % Add extra space after the heading -- half of whatever came above it. % Don't allow stretch, though. \kern .5 \csname #2headingskip\endcsname % % Do not let the kern be a potential breakpoint, as it would be if it % was followed by glue. \nobreak % % We'll almost certainly start a paragraph next, so don't let that % glue accumulate. (Not a breakpoint because it's preceded by a % discardable item.) However, when a paragraph is not started next % (\startdefun, \cartouche, \center, etc.), this needs to be wiped out % or the negative glue will cause weirdly wrong output, typically % obscuring the section heading with something else. \vskip-\parskip % % This is so the last item on the main vertical list is a known % \penalty > 10000, so \startdefun, etc., can recognize the situation % and do the needful. \penalty 10001 } \message{toc,} % Table of contents. \newwrite\tocfile % Write an entry to the toc file, opening it if necessary. % Called from @chapter, etc. % % Example usage: \writetocentry{sec}{Section Name}{\the\chapno.\the\secno} % We append the current node name (if any) and page number as additional % arguments for the \{chap,sec,...}entry macros which will eventually % read this. The node name is used in the pdf outlines as the % destination to jump to. % % We open the .toc file for writing here instead of at @setfilename (or % any other fixed time) so that @contents can be anywhere in the document. % But if #1 is `omit', then we don't do anything. This is used for the % table of contents chapter openings themselves. % \newif\iftocfileopened \def\omitkeyword{omit}% % \def\writetocentry#1#2#3{% \edef\writetoctype{#1}% \ifx\writetoctype\omitkeyword \else \iftocfileopened\else \immediate\openout\tocfile = \jobname.toc \global\tocfileopenedtrue \fi % \iflinks {\atdummies \edef\temp{% \write\tocfile{@#1entry{#2}{#3}{\lastnode}{\noexpand\folio}}}% \temp }% \fi \fi % % Tell \shipout to create a pdf destination on each page, if we're % writing pdf. These are used in the table of contents. We can't % just write one on every page because the title pages are numbered % 1 and 2 (the page numbers aren't printed), and so are the first % two pages of the document. Thus, we'd have two destinations named % `1', and two named `2'. \ifpdf \global\pdfmakepagedesttrue \else \ifx\XeTeXrevision\thisisundefined \else \global\pdfmakepagedesttrue \fi \fi } % These characters do not print properly in the Computer Modern roman % fonts, so we must take special care. This is more or less redundant % with the Texinfo input format setup at the end of this file. % \def\activecatcodes{% \catcode`\"=\active \catcode`\$=\active \catcode`\<=\active \catcode`\>=\active \catcode`\\=\active \catcode`\^=\active \catcode`\_=\active \catcode`\|=\active \catcode`\~=\active } % Read the toc file, which is essentially Texinfo input. \def\readtocfile{% \setupdatafile \activecatcodes \input \tocreadfilename } \newskip\contentsrightmargin \contentsrightmargin=1in \newcount\savepageno \newcount\lastnegativepageno \lastnegativepageno = -1 % Prepare to read what we've written to \tocfile. % \def\startcontents#1{% % If @setchapternewpage on, and @headings double, the contents should % start on an odd page, unlike chapters. Thus, we maintain % \contentsalignmacro in parallel with \pagealignmacro. % From: Torbjorn Granlund <tege@matematik.su.se> \contentsalignmacro \immediate\closeout\tocfile % % Don't need to put `Contents' or `Short Contents' in the headline. % It is abundantly clear what they are. \chapmacro{#1}{Yomitfromtoc}{}% % \savepageno = \pageno \begingroup % Set up to handle contents files properly. \raggedbottom % Worry more about breakpoints than the bottom. \entryrightmargin=\contentsrightmargin % Don't use the full line length. % % Roman numerals for page numbers. \ifnum \pageno>0 \global\pageno = \lastnegativepageno \fi } % redefined for the two-volume lispref. We always output on % \jobname.toc even if this is redefined. % \def\tocreadfilename{\jobname.toc} % Normal (long) toc. % \def\contents{% \startcontents{\putwordTOC}% \openin 1 \tocreadfilename\space \ifeof 1 \else \readtocfile \fi \vfill \eject \contentsalignmacro % in case @setchapternewpage odd is in effect \ifeof 1 \else \pdfmakeoutlines \fi \closein 1 \endgroup \lastnegativepageno = \pageno \global\pageno = \savepageno } % And just the chapters. \def\summarycontents{% \startcontents{\putwordShortTOC}% % \let\partentry = \shortpartentry \let\numchapentry = \shortchapentry \let\appentry = \shortchapentry \let\unnchapentry = \shortunnchapentry % We want a true roman here for the page numbers. \secfonts \let\rm=\shortcontrm \let\bf=\shortcontbf \let\sl=\shortcontsl \let\tt=\shortconttt \rm \hyphenpenalty = 10000 \advance\baselineskip by 1pt % Open it up a little. \def\numsecentry##1##2##3##4{} \let\appsecentry = \numsecentry \let\unnsecentry = \numsecentry \let\numsubsecentry = \numsecentry \let\appsubsecentry = \numsecentry \let\unnsubsecentry = \numsecentry \let\numsubsubsecentry = \numsecentry \let\appsubsubsecentry = \numsecentry \let\unnsubsubsecentry = \numsecentry \openin 1 \tocreadfilename\space \ifeof 1 \else \readtocfile \fi \closein 1 \vfill \eject \contentsalignmacro % in case @setchapternewpage odd is in effect \endgroup \lastnegativepageno = \pageno \global\pageno = \savepageno } \let\shortcontents = \summarycontents % Typeset the label for a chapter or appendix for the short contents. % The arg is, e.g., `A' for an appendix, or `3' for a chapter. % \def\shortchaplabel#1{% % This space should be enough, since a single number is .5em, and the % widest letter (M) is 1em, at least in the Computer Modern fonts. % But use \hss just in case. % (This space doesn't include the extra space that gets added after % the label; that gets put in by \shortchapentry above.) % % We'd like to right-justify chapter numbers, but that looks strange % with appendix letters. And right-justifying numbers and % left-justifying letters looks strange when there is less than 10 % chapters. Have to read the whole toc once to know how many chapters % there are before deciding ... \hbox to 1em{#1\hss}% } % These macros generate individual entries in the table of contents. % The first argument is the chapter or section name. % The last argument is the page number. % The arguments in between are the chapter number, section number, ... % Parts, in the main contents. Replace the part number, which doesn't % exist, with an empty box. Let's hope all the numbers have the same width. % Also ignore the page number, which is conventionally not printed. \def\numeralbox{\setbox0=\hbox{8}\hbox to \wd0{\hfil}} \def\partentry#1#2#3#4{% % Add stretch and a bonus for breaking the page before the part heading. % This reduces the chance of the page being broken immediately after the % part heading, before a following chapter heading. \vskip 0pt plus 5\baselineskip \penalty-300 \vskip 0pt plus -5\baselineskip \dochapentry{\numeralbox\labelspace#1}{}% } % % Parts, in the short toc. \def\shortpartentry#1#2#3#4{% \penalty-300 \vskip.5\baselineskip plus.15\baselineskip minus.1\baselineskip \shortchapentry{{\bf #1}}{\numeralbox}{}{}% } % Chapters, in the main contents. \def\numchapentry#1#2#3#4{\dochapentry{#2\labelspace#1}{#4}} % Chapters, in the short toc. % See comments in \dochapentry re vbox and related settings. \def\shortchapentry#1#2#3#4{% \tocentry{\shortchaplabel{#2}\labelspace #1}{\doshortpageno\bgroup#4\egroup}% } % Appendices, in the main contents. % Need the word Appendix, and a fixed-size box. % \def\appendixbox#1{% % We use M since it's probably the widest letter. \setbox0 = \hbox{\putwordAppendix{} M}% \hbox to \wd0{\putwordAppendix{} #1\hss}} % \def\appentry#1#2#3#4{\dochapentry{\appendixbox{#2}\hskip.7em#1}{#4}} % Unnumbered chapters. \def\unnchapentry#1#2#3#4{\dochapentry{#1}{#4}} \def\shortunnchapentry#1#2#3#4{\tocentry{#1}{\doshortpageno\bgroup#4\egroup}} % Sections. \def\numsecentry#1#2#3#4{\dosecentry{#2\labelspace#1}{#4}} \let\appsecentry=\numsecentry \def\unnsecentry#1#2#3#4{\dosecentry{#1}{#4}} % Subsections. \def\numsubsecentry#1#2#3#4{\dosubsecentry{#2\labelspace#1}{#4}} \let\appsubsecentry=\numsubsecentry \def\unnsubsecentry#1#2#3#4{\dosubsecentry{#1}{#4}} % And subsubsections. \def\numsubsubsecentry#1#2#3#4{\dosubsubsecentry{#2\labelspace#1}{#4}} \let\appsubsubsecentry=\numsubsubsecentry \def\unnsubsubsecentry#1#2#3#4{\dosubsubsecentry{#1}{#4}} % This parameter controls the indentation of the various levels. % Same as \defaultparindent. \newdimen\tocindent \tocindent = 15pt % Now for the actual typesetting. In all these, #1 is the text and #2 is the % page number. % % If the toc has to be broken over pages, we want it to be at chapters % if at all possible; hence the \penalty. \def\dochapentry#1#2{% \penalty-300 \vskip1\baselineskip plus.33\baselineskip minus.25\baselineskip \begingroup % Move the page numbers slightly to the right \advance\entryrightmargin by -0.05em \chapentryfonts \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup \nobreak\vskip .25\baselineskip plus.1\baselineskip } \def\dosecentry#1#2{\begingroup \secentryfonts \leftskip=\tocindent \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup} \def\dosubsecentry#1#2{\begingroup \subsecentryfonts \leftskip=2\tocindent \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup} \def\dosubsubsecentry#1#2{\begingroup \subsubsecentryfonts \leftskip=3\tocindent \tocentry{#1}{\dopageno\bgroup#2\egroup}% \endgroup} % We use the same \entry macro as for the index entries. \let\tocentry = \entry % Space between chapter (or whatever) number and the title. \def\labelspace{\hskip1em \relax} \def\dopageno#1{{\rm #1}} \def\doshortpageno#1{{\rm #1}} \def\chapentryfonts{\secfonts \rm} \def\secentryfonts{\textfonts} \def\subsecentryfonts{\textfonts} \def\subsubsecentryfonts{\textfonts} \message{environments,} % @foo ... @end foo. % @tex ... @end tex escapes into raw TeX temporarily. % One exception: @ is still an escape character, so that @end tex works. % But \@ or @@ will get a plain @ character. \envdef\tex{% \setupmarkupstyle{tex}% \catcode `\\=0 \catcode `\{=1 \catcode `\}=2 \catcode `\$=3 \catcode `\&=4 \catcode `\#=6 \catcode `\^=7 \catcode `\_=8 \catcode `\~=\active \let~=\tie \catcode `\%=14 \catcode `\+=\other \catcode `\"=\other \catcode `\|=\other \catcode `\<=\other \catcode `\>=\other \catcode `\`=\other \catcode `\'=\other % % ' is active in math mode (mathcode"8000). So reset it, and all our % other math active characters (just in case), to plain's definitions. \mathactive % % Inverse of the list at the beginning of the file. \let\b=\ptexb \let\bullet=\ptexbullet \let\c=\ptexc \let\,=\ptexcomma \let\.=\ptexdot \let\dots=\ptexdots \let\equiv=\ptexequiv \let\!=\ptexexclam \let\i=\ptexi \let\indent=\ptexindent \let\noindent=\ptexnoindent \let\{=\ptexlbrace \let\+=\tabalign \let\}=\ptexrbrace \let\/=\ptexslash \let\sp=\ptexsp \let\*=\ptexstar %\let\sup=\ptexsup % do not redefine, we want @sup to work in math mode \let\t=\ptext \expandafter \let\csname top\endcsname=\ptextop % we've made it outer \let\frenchspacing=\plainfrenchspacing % \def\endldots{\mathinner{\ldots\ldots\ldots\ldots}}% \def\enddots{\relax\ifmmode\endldots\else$\mathsurround=0pt \endldots\,$\fi}% \def\@{@}% } % There is no need to define \Etex. % Define @lisp ... @end lisp. % @lisp environment forms a group so it can rebind things, % including the definition of @end lisp (which normally is erroneous). % Amount to narrow the margins by for @lisp. \newskip\lispnarrowing \lispnarrowing=0.4in % This is the definition that ^^M gets inside @lisp, @example, and other % such environments. \null is better than a space, since it doesn't % have any width. \def\lisppar{\null\endgraf} % This space is always present above and below environments. \newskip\envskipamount \envskipamount = 0pt % Make spacing and below environment symmetrical. We use \parskip here % to help in doing that, since in @example-like environments \parskip % is reset to zero; thus the \afterenvbreak inserts no space -- but the % start of the next paragraph will insert \parskip. % \def\aboveenvbreak{{% % =10000 instead of <10000 because of a special case in \itemzzz and % \sectionheading, q.v. \ifnum \lastpenalty=10000 \else \advance\envskipamount by \parskip \endgraf \ifdim\lastskip<\envskipamount \removelastskip \ifnum\lastpenalty<10000 % Penalize breaking before the environment, because preceding text % often leads into it. \penalty100 \fi \vskip\envskipamount \fi \fi }} \def\afterenvbreak{{% % =10000 instead of <10000 because of a special case in \itemzzz and % \sectionheading, q.v. \ifnum \lastpenalty=10000 \else \advance\envskipamount by \parskip \endgraf \ifdim\lastskip<\envskipamount \removelastskip % it's not a good place to break if the last penalty was \nobreak % or better ... \ifnum\lastpenalty<10000 \penalty-50 \fi \vskip\envskipamount \fi \fi }} % \nonarrowing is a flag. If "set", @lisp etc don't narrow margins; it will % also clear it, so that its embedded environments do the narrowing again. \let\nonarrowing=\relax % @cartouche ... @end cartouche: draw rectangle w/rounded corners around % environment contents. \font\circle=lcircle10 \newdimen\circthick \newdimen\cartouter\newdimen\cartinner \newskip\normbskip\newskip\normpskip\newskip\normlskip \circthick=\fontdimen8\circle % \def\ctl{{\circle\char'013\hskip -6pt}}% 6pt from pl file: 1/2charwidth \def\ctr{{\hskip 6pt\circle\char'010}} \def\cbl{{\circle\char'012\hskip -6pt}} \def\cbr{{\hskip 6pt\circle\char'011}} \def\carttop{\hbox to \cartouter{\hskip\lskip \ctl\leaders\hrule height\circthick\hfil\ctr \hskip\rskip}} \def\cartbot{\hbox to \cartouter{\hskip\lskip \cbl\leaders\hrule height\circthick\hfil\cbr \hskip\rskip}} % \newskip\lskip\newskip\rskip \envdef\cartouche{% \ifhmode\par\fi % can't be in the midst of a paragraph. \startsavinginserts \lskip=\leftskip \rskip=\rightskip \leftskip=0pt\rightskip=0pt % we want these *outside*. \cartinner=\hsize \advance\cartinner by-\lskip \advance\cartinner by-\rskip \cartouter=\hsize \advance\cartouter by 18.4pt % allow for 3pt kerns on either % side, and for 6pt waste from % each corner char, and rule thickness \normbskip=\baselineskip \normpskip=\parskip \normlskip=\lineskip % % If this cartouche directly follows a sectioning command, we need the % \parskip glue (backspaced over by default) or the cartouche can % collide with the section heading. \ifnum\lastpenalty>10000 \vskip\parskip \penalty\lastpenalty \fi % \setbox\groupbox=\vbox\bgroup \baselineskip=0pt\parskip=0pt\lineskip=0pt \carttop \hbox\bgroup \hskip\lskip \vrule\kern3pt \vbox\bgroup \kern3pt \hsize=\cartinner \baselineskip=\normbskip \lineskip=\normlskip \parskip=\normpskip \vskip -\parskip \comment % For explanation, see the end of def\group. } \def\Ecartouche{% \ifhmode\par\fi \kern3pt \egroup \kern3pt\vrule \hskip\rskip \egroup \cartbot \egroup \addgroupbox \checkinserts } % This macro is called at the beginning of all the @example variants, % inside a group. \newdimen\nonfillparindent \def\nonfillstart{% \aboveenvbreak \ifdim\hfuzz < 12pt \hfuzz = 12pt \fi % Don't be fussy \sepspaces % Make spaces be word-separators rather than space tokens. \let\par = \lisppar % don't ignore blank lines \obeylines % each line of input is a line of output \parskip = 0pt % Turn off paragraph indentation but redefine \indent to emulate % the normal \indent. \nonfillparindent=\parindent \parindent = 0pt \let\indent\nonfillindent % \emergencystretch = 0pt % don't try to avoid overfull boxes \ifx\nonarrowing\relax \advance \leftskip by \lispnarrowing \exdentamount=\lispnarrowing \else \let\nonarrowing = \relax \fi \let\exdent=\nofillexdent } \begingroup \obeyspaces % We want to swallow spaces (but not other tokens) after the fake % @indent in our nonfill-environments, where spaces are normally % active and set to @tie, resulting in them not being ignored after % @indent. \gdef\nonfillindent{\futurelet\temp\nonfillindentcheck}% \gdef\nonfillindentcheck{% \ifx\temp % \expandafter\nonfillindentgobble% \else% \leavevmode\nonfillindentbox% \fi% }% \endgroup \def\nonfillindentgobble#1{\nonfillindent} \def\nonfillindentbox{\hbox to \nonfillparindent{\hss}} % If you want all examples etc. small: @set dispenvsize small. % If you want even small examples the full size: @set dispenvsize nosmall. % This affects the following displayed environments: % @example, @display, @format, @lisp % \def\smallword{small} \def\nosmallword{nosmall} \let\SETdispenvsize\relax \def\setnormaldispenv{% \ifx\SETdispenvsize\smallword % end paragraph for sake of leading, in case document has no blank % line. This is redundant with what happens in \aboveenvbreak, but % we need to do it before changing the fonts, and it's inconvenient % to change the fonts afterward. \ifnum \lastpenalty=10000 \else \endgraf \fi \smallexamplefonts \rm \fi } \def\setsmalldispenv{% \ifx\SETdispenvsize\nosmallword \else \ifnum \lastpenalty=10000 \else \endgraf \fi \smallexamplefonts \rm \fi } % We often define two environments, @foo and @smallfoo. % Let's do it in one command. #1 is the env name, #2 the definition. \def\makedispenvdef#1#2{% \expandafter\envdef\csname#1\endcsname {\setnormaldispenv #2}% \expandafter\envdef\csname small#1\endcsname {\setsmalldispenv #2}% \expandafter\let\csname E#1\endcsname \afterenvbreak \expandafter\let\csname Esmall#1\endcsname \afterenvbreak } % Define two environment synonyms (#1 and #2) for an environment. \def\maketwodispenvdef#1#2#3{% \makedispenvdef{#1}{#3}% \makedispenvdef{#2}{#3}% } % % @lisp: indented, narrowed, typewriter font; % @example: same as @lisp. % % @smallexample and @smalllisp: use smaller fonts. % Originally contributed by Pavel@xerox. % \maketwodispenvdef{lisp}{example}{% \nonfillstart \tt\setupmarkupstyle{example}% \let\kbdfont = \kbdexamplefont % Allow @kbd to do something special. \gobble % eat return } % @display/@smalldisplay: same as @lisp except keep current font. % \makedispenvdef{display}{% \nonfillstart \gobble } % @format/@smallformat: same as @display except don't narrow margins. % \makedispenvdef{format}{% \let\nonarrowing = t% \nonfillstart \gobble } % @flushleft: same as @format, but doesn't obey \SETdispenvsize. \envdef\flushleft{% \let\nonarrowing = t% \nonfillstart \gobble } \let\Eflushleft = \afterenvbreak % @flushright. % \envdef\flushright{% \let\nonarrowing = t% \nonfillstart \advance\leftskip by 0pt plus 1fill\relax \gobble } \let\Eflushright = \afterenvbreak % @raggedright does more-or-less normal line breaking but no right % justification. From plain.tex. Don't stretch around special % characters in urls in this environment, since the stretch at the right % should be enough. \envdef\raggedright{% \rightskip0pt plus2.4em \spaceskip.3333em \xspaceskip.5em\relax \def\urefprestretchamount{0pt}% \def\urefpoststretchamount{0pt}% } \let\Eraggedright\par \envdef\raggedleft{% \parindent=0pt \leftskip0pt plus2em \spaceskip.3333em \xspaceskip.5em \parfillskip=0pt \hbadness=10000 % Last line will usually be underfull, so turn off % badness reporting. } \let\Eraggedleft\par \envdef\raggedcenter{% \parindent=0pt \rightskip0pt plus1em \leftskip0pt plus1em \spaceskip.3333em \xspaceskip.5em \parfillskip=0pt \hbadness=10000 % Last line will usually be underfull, so turn off % badness reporting. } \let\Eraggedcenter\par % @quotation does normal linebreaking (hence we can't use \nonfillstart) % and narrows the margins. We keep \parskip nonzero in general, since % we're doing normal filling. So, when using \aboveenvbreak and % \afterenvbreak, temporarily make \parskip 0. % \makedispenvdef{quotation}{\quotationstart} % \def\quotationstart{% \indentedblockstart % same as \indentedblock, but increase right margin too. \ifx\nonarrowing\relax \advance\rightskip by \lispnarrowing \fi \parsearg\quotationlabel } % We have retained a nonzero parskip for the environment, since we're % doing normal filling. % \def\Equotation{% \par \ifx\quotationauthor\thisisundefined\else % indent a bit. \leftline{\kern 2\leftskip \sl ---\quotationauthor}% \fi {\parskip=0pt \afterenvbreak}% } \def\Esmallquotation{\Equotation} % If we're given an argument, typeset it in bold with a colon after. \def\quotationlabel#1{% \def\temp{#1}% \ifx\temp\empty \else {\bf #1: }% \fi } % @indentedblock is like @quotation, but indents only on the left and % has no optional argument. % \makedispenvdef{indentedblock}{\indentedblockstart} % \def\indentedblockstart{% {\parskip=0pt \aboveenvbreak}% because \aboveenvbreak inserts \parskip \parindent=0pt % % @cartouche defines \nonarrowing to inhibit narrowing at next level down. \ifx\nonarrowing\relax \advance\leftskip by \lispnarrowing \exdentamount = \lispnarrowing \else \let\nonarrowing = \relax \fi } % Keep a nonzero parskip for the environment, since we're doing normal filling. % \def\Eindentedblock{% \par {\parskip=0pt \afterenvbreak}% } \def\Esmallindentedblock{\Eindentedblock} % LaTeX-like @verbatim...@end verbatim and @verb{<char>...<char>} % If we want to allow any <char> as delimiter, % we need the curly braces so that makeinfo sees the @verb command, eg: % `@verbx...x' would look like the '@verbx' command. --janneke@gnu.org % % [Knuth]: Donald Ervin Knuth, 1996. The TeXbook. % % [Knuth] p.344; only we need to do the other characters Texinfo sets % active too. Otherwise, they get lost as the first character on a % verbatim line. \def\dospecials{% \do\ \do\\\do\{\do\}\do\$\do\&% \do\#\do\^\do\^^K\do\_\do\^^A\do\%\do\~% \do\<\do\>\do\|\do\@\do+\do\"% % Don't do the quotes -- if we do, @set txicodequoteundirected and % @set txicodequotebacktick will not have effect on @verb and % @verbatim, and ?` and !` ligatures won't get disabled. %\do\`\do\'% } % % [Knuth] p. 380 \def\uncatcodespecials{% \def\do##1{\catcode`##1=\other}\dospecials} % % Setup for the @verb command. % % Eight spaces for a tab \begingroup \catcode`\^^I=\active \gdef\tabeightspaces{\catcode`\^^I=\active\def^^I{\ \ \ \ \ \ \ \ }} \endgroup % \def\setupverb{% \tt % easiest (and conventionally used) font for verbatim \def\par{\leavevmode\endgraf}% \setupmarkupstyle{verb}% \tabeightspaces % Respect line breaks, % print special symbols as themselves, and % make each space count % must do in this order: \obeylines \uncatcodespecials \sepspaces } % Setup for the @verbatim environment % % Real tab expansion. \newdimen\tabw \setbox0=\hbox{\tt\space} \tabw=8\wd0 % tab amount % % We typeset each line of the verbatim in an \hbox, so we can handle % tabs. The \global is in case the verbatim line starts with an accent, % or some other command that starts with a begin-group. Otherwise, the % entire \verbbox would disappear at the corresponding end-group, before % it is typeset. Meanwhile, we can't have nested verbatim commands % (can we?), so the \global won't be overwriting itself. \newbox\verbbox \def\starttabbox{\global\setbox\verbbox=\hbox\bgroup} % \begingroup \catcode`\^^I=\active \gdef\tabexpand{% \catcode`\^^I=\active \def^^I{\leavevmode\egroup \dimen\verbbox=\wd\verbbox % the width so far, or since the previous tab \divide\dimen\verbbox by\tabw \multiply\dimen\verbbox by\tabw % compute previous multiple of \tabw \advance\dimen\verbbox by\tabw % advance to next multiple of \tabw \wd\verbbox=\dimen\verbbox \box\verbbox \starttabbox }% } \endgroup % start the verbatim environment. \def\setupverbatim{% \let\nonarrowing = t% \nonfillstart \tt % easiest (and conventionally used) font for verbatim % The \leavevmode here is for blank lines. Otherwise, we would % never \starttabox and the \egroup would end verbatim mode. \def\par{\leavevmode\egroup\box\verbbox\endgraf}% \tabexpand \setupmarkupstyle{verbatim}% % Respect line breaks, % print special symbols as themselves, and % make each space count. % Must do in this order: \obeylines \uncatcodespecials \sepspaces \everypar{\starttabbox}% } % Do the @verb magic: verbatim text is quoted by unique % delimiter characters. Before first delimiter expect a % right brace, after last delimiter expect closing brace: % % \def\doverb'{'<char>#1<char>'}'{#1} % % [Knuth] p. 382; only eat outer {} \begingroup \catcode`[=1\catcode`]=2\catcode`\{=\other\catcode`\}=\other \gdef\doverb{#1[\def\next##1#1}[##1\endgroup]\next] \endgroup % \def\verb{\begingroup\setupverb\doverb} % % % Do the @verbatim magic: define the macro \doverbatim so that % the (first) argument ends when '@end verbatim' is reached, ie: % % \def\doverbatim#1@end verbatim{#1} % % For Texinfo it's a lot easier than for LaTeX, % because texinfo's \verbatim doesn't stop at '\end{verbatim}': % we need not redefine '\', '{' and '}'. % % Inspired by LaTeX's verbatim command set [latex.ltx] % \begingroup \catcode`\ =\active \obeylines % % ignore everything up to the first ^^M, that's the newline at the end % of the @verbatim input line itself. Otherwise we get an extra blank % line in the output. \xdef\doverbatim#1^^M#2@end verbatim{#2\noexpand\end\gobble verbatim}% % We really want {...\end verbatim} in the body of the macro, but % without the active space; thus we have to use \xdef and \gobble. \endgroup % \envdef\verbatim{% \setupverbatim\doverbatim } \let\Everbatim = \afterenvbreak % @verbatiminclude FILE - insert text of file in verbatim environment. % \def\verbatiminclude{\parseargusing\filenamecatcodes\doverbatiminclude} % \def\doverbatiminclude#1{% {% \makevalueexpandable \setupverbatim \indexnofonts % Allow `@@' and other weird things in file names. \wlog{texinfo.tex: doing @verbatiminclude of #1^^J}% \input #1 \afterenvbreak }% } % @copying ... @end copying. % Save the text away for @insertcopying later. % % We save the uninterpreted tokens, rather than creating a box. % Saving the text in a box would be much easier, but then all the % typesetting commands (@smallbook, font changes, etc.) have to be done % beforehand -- and a) we want @copying to be done first in the source % file; b) letting users define the frontmatter in as flexible order as % possible is desirable. % \def\copying{\checkenv{}\begingroup\scanargctxt\docopying} \def\docopying#1@end copying{\endgroup\def\copyingtext{#1}} % \def\insertcopying{% \begingroup \parindent = 0pt % paragraph indentation looks wrong on title page \scanexp\copyingtext \endgroup } \message{defuns,} % @defun etc. \newskip\defbodyindent \defbodyindent=.4in \newskip\defargsindent \defargsindent=50pt \newskip\deflastargmargin \deflastargmargin=18pt \newcount\defunpenalty % Start the processing of @deffn: \def\startdefun{% \ifnum\lastpenalty<10000 \medbreak \defunpenalty=10003 % Will keep this @deffn together with the % following @def command, see below. \else % If there are two @def commands in a row, we'll have a \nobreak, % which is there to keep the function description together with its % header. But if there's nothing but headers, we need to allow a % break somewhere. Check specifically for penalty 10002, inserted % by \printdefunline, instead of 10000, since the sectioning % commands also insert a nobreak penalty, and we don't want to allow % a break between a section heading and a defun. % % As a further refinement, we avoid "club" headers by signalling % with penalty of 10003 after the very first @deffn in the % sequence (see above), and penalty of 10002 after any following % @def command. \ifnum\lastpenalty=10002 \penalty2000 \else \defunpenalty=10002 \fi % % Similarly, after a section heading, do not allow a break. % But do insert the glue. \medskip % preceded by discardable penalty, so not a breakpoint \fi % \parindent=0in \advance\leftskip by \defbodyindent \exdentamount=\defbodyindent } \def\dodefunx#1{% % First, check whether we are in the right environment: \checkenv#1% % % As above, allow line break if we have multiple x headers in a row. % It's not a great place, though. \ifnum\lastpenalty=10002 \penalty3000 \else \defunpenalty=10002 \fi % % And now, it's time to reuse the body of the original defun: \expandafter\gobbledefun#1% } \def\gobbledefun#1\startdefun{} % \printdefunline \deffnheader{text} % \def\printdefunline#1#2{% \begingroup % call \deffnheader: #1#2 \endheader % common ending: \interlinepenalty = 10000 \advance\rightskip by 0pt plus 1fil\relax \endgraf \nobreak\vskip -\parskip \penalty\defunpenalty % signal to \startdefun and \dodefunx % Some of the @defun-type tags do not enable magic parentheses, % rendering the following check redundant. But we don't optimize. \checkparencounts \endgroup } \def\Edefun{\endgraf\medbreak} % \makedefun{deffn} creates \deffn, \deffnx and \Edeffn; % the only thing remaining is to define \deffnheader. % \def\makedefun#1{% \expandafter\let\csname E#1\endcsname = \Edefun \edef\temp{\noexpand\domakedefun \makecsname{#1}\makecsname{#1x}\makecsname{#1header}}% \temp } % \domakedefun \deffn \deffnx \deffnheader { (defn. of \deffnheader) } % % Define \deffn and \deffnx, without parameters. % \deffnheader has to be defined explicitly. % \def\domakedefun#1#2#3{% \envdef#1{% \startdefun \doingtypefnfalse % distinguish typed functions from all else \parseargusing\activeparens{\printdefunline#3}% }% \def#2{\dodefunx#1}% \def#3% } \newif\ifdoingtypefn % doing typed function? \newif\ifrettypeownline % typeset return type on its own line? % @deftypefnnewline on|off says whether the return type of typed functions % are printed on their own line. This affects @deftypefn, @deftypefun, % @deftypeop, and @deftypemethod. % \parseargdef\deftypefnnewline{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETtxideftypefnnl\endcsname = \empty \else\ifx\temp\offword \expandafter\let\csname SETtxideftypefnnl\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @txideftypefnnl value `\temp', must be on|off}% \fi\fi } % Untyped functions: % @deffn category name args \makedefun{deffn}{\deffngeneral{}} % @deffn category class name args \makedefun{defop}#1 {\defopon{#1\ \putwordon}} % \defopon {category on}class name args \def\defopon#1#2 {\deffngeneral{\putwordon\ \code{#2}}{#1\ \code{#2}} } % \deffngeneral {subind}category name args % \def\deffngeneral#1#2 #3 #4\endheader{% % Remember that \dosubind{fn}{foo}{} is equivalent to \doind{fn}{foo}. \dosubind{fn}{\code{#3}}{#1}% \defname{#2}{}{#3}\magicamp\defunargs{#4\unskip}% } % Typed functions: % @deftypefn category type name args \makedefun{deftypefn}{\deftypefngeneral{}} % @deftypeop category class type name args \makedefun{deftypeop}#1 {\deftypeopon{#1\ \putwordon}} % \deftypeopon {category on}class type name args \def\deftypeopon#1#2 {\deftypefngeneral{\putwordon\ \code{#2}}{#1\ \code{#2}} } % \deftypefngeneral {subind}category type name args % \def\deftypefngeneral#1#2 #3 #4 #5\endheader{% \dosubind{fn}{\code{#4}}{#1}% \doingtypefntrue \defname{#2}{#3}{#4}\defunargs{#5\unskip}% } % Typed variables: % @deftypevr category type var args \makedefun{deftypevr}{\deftypecvgeneral{}} % @deftypecv category class type var args \makedefun{deftypecv}#1 {\deftypecvof{#1\ \putwordof}} % \deftypecvof {category of}class type var args \def\deftypecvof#1#2 {\deftypecvgeneral{\putwordof\ \code{#2}}{#1\ \code{#2}} } % \deftypecvgeneral {subind}category type var args % \def\deftypecvgeneral#1#2 #3 #4 #5\endheader{% \dosubind{vr}{\code{#4}}{#1}% \defname{#2}{#3}{#4}\defunargs{#5\unskip}% } % Untyped variables: % @defvr category var args \makedefun{defvr}#1 {\deftypevrheader{#1} {} } % @defcv category class var args \makedefun{defcv}#1 {\defcvof{#1\ \putwordof}} % \defcvof {category of}class var args \def\defcvof#1#2 {\deftypecvof{#1}#2 {} } % Types: % @deftp category name args \makedefun{deftp}#1 #2 #3\endheader{% \doind{tp}{\code{#2}}% \defname{#1}{}{#2}\defunargs{#3\unskip}% } % Remaining @defun-like shortcuts: \makedefun{defun}{\deffnheader{\putwordDeffunc} } \makedefun{defmac}{\deffnheader{\putwordDefmac} } \makedefun{defspec}{\deffnheader{\putwordDefspec} } \makedefun{deftypefun}{\deftypefnheader{\putwordDeffunc} } \makedefun{defvar}{\defvrheader{\putwordDefvar} } \makedefun{defopt}{\defvrheader{\putwordDefopt} } \makedefun{deftypevar}{\deftypevrheader{\putwordDefvar} } \makedefun{defmethod}{\defopon\putwordMethodon} \makedefun{deftypemethod}{\deftypeopon\putwordMethodon} \makedefun{defivar}{\defcvof\putwordInstanceVariableof} \makedefun{deftypeivar}{\deftypecvof\putwordInstanceVariableof} % \defname, which formats the name of the @def (not the args). % #1 is the category, such as "Function". % #2 is the return type, if any. % #3 is the function name. % % We are followed by (but not passed) the arguments, if any. % \def\defname#1#2#3{% \par % Get the values of \leftskip and \rightskip as they were outside the @def... \advance\leftskip by -\defbodyindent % % Determine if we are typesetting the return type of a typed function % on a line by itself. \rettypeownlinefalse \ifdoingtypefn % doing a typed function specifically? % then check user option for putting return type on its own line: \expandafter\ifx\csname SETtxideftypefnnl\endcsname\relax \else \rettypeownlinetrue \fi \fi % % How we'll format the category name. Putting it in brackets helps % distinguish it from the body text that may end up on the next line % just below it. \def\temp{#1}% \setbox0=\hbox{\kern\deflastargmargin \ifx\temp\empty\else [\rm\temp]\fi} % % Figure out line sizes for the paragraph shape. We'll always have at % least two. \tempnum = 2 % % The first line needs space for \box0; but if \rightskip is nonzero, % we need only space for the part of \box0 which exceeds it: \dimen0=\hsize \advance\dimen0 by -\wd0 \advance\dimen0 by \rightskip % % If doing a return type on its own line, we'll have another line. \ifrettypeownline \advance\tempnum by 1 \def\maybeshapeline{0in \hsize}% \else \def\maybeshapeline{}% \fi % % The continuations: \dimen2=\hsize \advance\dimen2 by -\defargsindent % % The final paragraph shape: \parshape \tempnum 0in \dimen0 \maybeshapeline \defargsindent \dimen2 % % Put the category name at the right margin. \noindent \hbox to 0pt{% \hfil\box0 \kern-\hsize % \hsize has to be shortened this way: \kern\leftskip % Intentionally do not respect \rightskip, since we need the space. }% % % Allow all lines to be underfull without complaint: \tolerance=10000 \hbadness=10000 \exdentamount=\defbodyindent {% % defun fonts. We use typewriter by default (used to be bold) because: % . we're printing identifiers, they should be in tt in principle. % . in languages with many accents, such as Czech or French, it's % common to leave accents off identifiers. The result looks ok in % tt, but exceedingly strange in rm. % . we don't want -- and --- to be treated as ligatures. % . this still does not fix the ?` and !` ligatures, but so far no % one has made identifiers using them :). \df \tt \def\temp{#2}% text of the return type \ifx\temp\empty\else \tclose{\temp}% typeset the return type \ifrettypeownline % put return type on its own line; prohibit line break following: \hfil\vadjust{\nobreak}\break \else \space % type on same line, so just followed by a space \fi \fi % no return type #3% output function name }% {\rm\enskip}% hskip 0.5 em of \rmfont % \boldbrax % arguments will be output next, if any. } % Print arguments in slanted roman (not ttsl), inconsistently with using % tt for the name. This is because literal text is sometimes needed in % the argument list (groff manual), and ttsl and tt are not very % distinguishable. Prevent hyphenation at `-' chars. % \def\defunargs#1{% % use sl by default (not ttsl), % tt for the names. \df \sl \hyphenchar\font=0 % % On the other hand, if an argument has two dashes (for instance), we % want a way to get ttsl. We used to recommend @var for that, so % leave the code in, but it's strange for @var to lead to typewriter. % Nowadays we recommend @code, since the difference between a ttsl hyphen % and a tt hyphen is pretty tiny. @code also disables ?` !`. \def\var##1{{\setupmarkupstyle{var}\ttslanted{##1}}}% #1% \sl\hyphenchar\font=45 } % We want ()&[] to print specially on the defun line. % \def\activeparens{% \catcode`\(=\active \catcode`\)=\active \catcode`\[=\active \catcode`\]=\active \catcode`\&=\active } % Make control sequences which act like normal parenthesis chars. \let\lparen = ( \let\rparen = ) % Be sure that we always have a definition for `(', etc. For example, % if the fn name has parens in it, \boldbrax will not be in effect yet, % so TeX would otherwise complain about undefined control sequence. { \activeparens \global\let(=\lparen \global\let)=\rparen \global\let[=\lbrack \global\let]=\rbrack \global\let& = \& \gdef\boldbrax{\let(=\opnr\let)=\clnr\let[=\lbrb\let]=\rbrb} \gdef\magicamp{\let&=\amprm} } \newcount\parencount % If we encounter &foo, then turn on ()-hacking afterwards \newif\ifampseen \def\amprm#1 {\ampseentrue{\bf\ }} \def\parenfont{% \ifampseen % At the first level, print parens in roman, % otherwise use the default font. \ifnum \parencount=1 \rm \fi \else % The \sf parens (in \boldbrax) actually are a little bolder than % the contained text. This is especially needed for [ and ] . \sf \fi } \def\infirstlevel#1{% \ifampseen \ifnum\parencount=1 #1% \fi \fi } \def\bfafterword#1 {#1 \bf} \def\opnr{% \global\advance\parencount by 1 {\parenfont(}% \infirstlevel \bfafterword } \def\clnr{% {\parenfont)}% \infirstlevel \sl \global\advance\parencount by -1 } \newcount\brackcount \def\lbrb{% \global\advance\brackcount by 1 {\bf[}% } \def\rbrb{% {\bf]}% \global\advance\brackcount by -1 } \def\checkparencounts{% \ifnum\parencount=0 \else \badparencount \fi \ifnum\brackcount=0 \else \badbrackcount \fi } % these should not use \errmessage; the glibc manual, at least, actually % has such constructs (when documenting function pointers). \def\badparencount{% \message{Warning: unbalanced parentheses in @def...}% \global\parencount=0 } \def\badbrackcount{% \message{Warning: unbalanced square brackets in @def...}% \global\brackcount=0 } \message{macros,} % @macro. % To do this right we need a feature of e-TeX, \scantokens, % which we arrange to emulate with a temporary file in ordinary TeX. \ifx\eTeXversion\thisisundefined \newwrite\macscribble \def\scantokens#1{% \toks0={#1}% \immediate\openout\macscribble=\jobname.tmp \immediate\write\macscribble{\the\toks0}% \immediate\closeout\macscribble \input \jobname.tmp } \fi % alias because \c means cedilla in @tex or @math \let\texinfoc=\c \newcount\savedcatcodeone \newcount\savedcatcodetwo % Used at the time of macro expansion. % Argument is macro body with arguments substituted \def\scanmacro#1{% \newlinechar`\^^M \def\xeatspaces{\eatspaces}% % % Temporarily undo catcode changes of \printindex. Set catcode of @ to % 0 so that @-commands in macro expansions aren't printed literally when % formatting an index file, where \ is used as the escape character. \savedcatcodeone=\catcode`\@ \savedcatcodetwo=\catcode`\\ \catcode`\@=0 \catcode`\\=\active % % Process the macro body under the current catcode regime. \scantokens{#1@texinfoc}% % \catcode`\@=\savedcatcodeone \catcode`\\=\savedcatcodetwo % % The \texinfoc is to remove the \newlinechar added by \scantokens, and % can be noticed by \parsearg. % We avoid surrounding the call to \scantokens with \bgroup and \egroup % to allow macros to open or close groups themselves. } % Used for copying and captions \def\scanexp#1{% \expandafter\scanmacro\expandafter{#1}% } \newcount\paramno % Count of parameters \newtoks\macname % Macro name \newif\ifrecursive % Is it recursive? % List of all defined macros in the form % \commondummyword\macro1\commondummyword\macro2... % Currently is also contains all @aliases; the list can be split % if there is a need. \def\macrolist{} % Add the macro to \macrolist \def\addtomacrolist#1{\expandafter \addtomacrolistxxx \csname#1\endcsname} \def\addtomacrolistxxx#1{% \toks0 = \expandafter{\macrolist\commondummyword#1}% \xdef\macrolist{\the\toks0}% } % Utility routines. % This does \let #1 = #2, with \csnames; that is, % \let \csname#1\endcsname = \csname#2\endcsname % (except of course we have to play expansion games). % \def\cslet#1#2{% \expandafter\let \csname#1\expandafter\endcsname \csname#2\endcsname } % Trim leading and trailing spaces off a string. % Concepts from aro-bend problem 15 (see CTAN). {\catcode`\@=11 \gdef\eatspaces #1{\expandafter\trim@\expandafter{#1 }} \gdef\trim@ #1{\trim@@ @#1 @ #1 @ @@} \gdef\trim@@ #1@ #2@ #3@@{\trim@@@\empty #2 @} \def\unbrace#1{#1} \unbrace{\gdef\trim@@@ #1 } #2@{#1} } % Trim a single trailing ^^M off a string. {\catcode`\^^M=\other \catcode`\Q=3% \gdef\eatcr #1{\eatcra #1Q^^MQ}% \gdef\eatcra#1^^MQ{\eatcrb#1Q}% \gdef\eatcrb#1Q#2Q{#1}% } % Macro bodies are absorbed as an argument in a context where % all characters are catcode 10, 11 or 12, except \ which is active % (as in normal texinfo). It is necessary to change the definition of \ % to recognize macro arguments; this is the job of \mbodybackslash. % % Non-ASCII encodings make 8-bit characters active, so un-activate % them to avoid their expansion. Must do this non-globally, to % confine the change to the current group. % % It's necessary to have hard CRs when the macro is executed. This is % done by making ^^M (\endlinechar) catcode 12 when reading the macro % body, and then making it the \newlinechar in \scanmacro. % \def\scanctxt{% used as subroutine \catcode`\"=\other \catcode`\+=\other \catcode`\<=\other \catcode`\>=\other \catcode`\^=\other \catcode`\_=\other \catcode`\|=\other \catcode`\~=\other \passthroughcharstrue } \def\scanargctxt{% used for copying and captions, not macros. \scanctxt \catcode`\@=\other \catcode`\\=\other \catcode`\^^M=\other } \def\macrobodyctxt{% used for @macro definitions \scanctxt \catcode`\ =\other \catcode`\@=\other \catcode`\{=\other \catcode`\}=\other \catcode`\^^M=\other \usembodybackslash } % Used when scanning braced macro arguments. Note, however, that catcode % changes here are ineffectual if the macro invocation was nested inside % an argument to another Texinfo command. \def\macroargctxt{% \scanctxt \catcode`\ =\active \catcode`\^^M=\other \catcode`\\=\active } \def\macrolineargctxt{% used for whole-line arguments without braces \scanctxt \catcode`\{=\other \catcode`\}=\other } % \mbodybackslash is the definition of \ in @macro bodies. % It maps \foo\ => \csname macarg.foo\endcsname => #N % where N is the macro parameter number. % We define \csname macarg.\endcsname to be \realbackslash, so % \\ in macro replacement text gets you a backslash. % {\catcode`@=0 @catcode`@\=@active @gdef@usembodybackslash{@let\=@mbodybackslash} @gdef@mbodybackslash#1\{@csname macarg.#1@endcsname} } \expandafter\def\csname macarg.\endcsname{\realbackslash} \def\margbackslash#1{\char`\#1 } \def\macro{\recursivefalse\parsearg\macroxxx} \def\rmacro{\recursivetrue\parsearg\macroxxx} \def\macroxxx#1{% \getargs{#1}% now \macname is the macname and \argl the arglist \ifx\argl\empty % no arguments \paramno=0\relax \else \expandafter\parsemargdef \argl;% \if\paramno>256\relax \ifx\eTeXversion\thisisundefined \errhelp = \EMsimple \errmessage{You need eTeX to compile a file with macros with more than 256 arguments} \fi \fi \fi \if1\csname ismacro.\the\macname\endcsname \message{Warning: redefining \the\macname}% \else \expandafter\ifx\csname \the\macname\endcsname \relax \else \errmessage{Macro name \the\macname\space already defined}\fi \global\cslet{macsave.\the\macname}{\the\macname}% \global\expandafter\let\csname ismacro.\the\macname\endcsname=1% \addtomacrolist{\the\macname}% \fi \begingroup \macrobodyctxt \ifrecursive \expandafter\parsermacbody \else \expandafter\parsemacbody \fi} \parseargdef\unmacro{% \if1\csname ismacro.#1\endcsname \global\cslet{#1}{macsave.#1}% \global\expandafter\let \csname ismacro.#1\endcsname=0% % Remove the macro name from \macrolist: \begingroup \expandafter\let\csname#1\endcsname \relax \let\commondummyword\unmacrodo \xdef\macrolist{\macrolist}% \endgroup \else \errmessage{Macro #1 not defined}% \fi } % Called by \do from \dounmacro on each macro. The idea is to omit any % macro definitions that have been changed to \relax. % \def\unmacrodo#1{% \ifx #1\relax % remove this \else \noexpand\commondummyword \noexpand#1% \fi } % \getargs -- Parse the arguments to a @macro line. Set \macname to % the name of the macro, and \argl to the braced argument list. \def\getargs#1{\getargsxxx#1{}} \def\getargsxxx#1#{\getmacname #1 \relax\getmacargs} \def\getmacname#1 #2\relax{\macname={#1}} \def\getmacargs#1{\def\argl{#1}} % This made use of the feature that if the last token of a % <parameter list> is #, then the preceding argument is delimited by % an opening brace, and that opening brace is not consumed. % Parse the optional {params} list to @macro or @rmacro. % Set \paramno to the number of arguments, % and \paramlist to a parameter text for the macro (e.g. #1,#2,#3 for a % three-param macro.) Define \macarg.BLAH for each BLAH in the params % list to some hook where the argument is to be expanded. If there are % less than 10 arguments that hook is to be replaced by ##N where N % is the position in that list, that is to say the macro arguments are to be % defined `a la TeX in the macro body. % % That gets used by \mbodybackslash (above). % % If there are 10 or more arguments, a different technique is used: see % \parsemmanyargdef. % \def\parsemargdef#1;{% \paramno=0\def\paramlist{}% \let\hash\relax % \hash is redefined to `#' later to get it into definitions \let\xeatspaces\relax \parsemargdefxxx#1,;,% \ifnum\paramno<10\relax\else \paramno0\relax \parsemmanyargdef@@#1,;,% 10 or more arguments \fi } \def\parsemargdefxxx#1,{% \if#1;\let\next=\relax \else \let\next=\parsemargdefxxx \advance\paramno by 1 \expandafter\edef\csname macarg.\eatspaces{#1}\endcsname {\xeatspaces{\hash\the\paramno}}% \edef\paramlist{\paramlist\hash\the\paramno,}% \fi\next} % \parsemacbody, \parsermacbody % % Read recursive and nonrecursive macro bodies. (They're different since % rec and nonrec macros end differently.) % % We are in \macrobodyctxt, and the \xdef causes backslashshes in the macro % body to be transformed. % Set \macrobody to the body of the macro, and call \defmacro. % {\catcode`\ =\other\long\gdef\parsemacbody#1@end macro{% \xdef\macrobody{\eatcr{#1}}\endgroup\defmacro}}% {\catcode`\ =\other\long\gdef\parsermacbody#1@end rmacro{% \xdef\macrobody{\eatcr{#1}}\endgroup\defmacro}}% % Make @ a letter, so that we can make private-to-Texinfo macro names. \edef\texiatcatcode{\the\catcode`\@} \catcode `@=11\relax %%%%%%%%%%%%%% Code for > 10 arguments only %%%%%%%%%%%%%%%%%% % If there are 10 or more arguments, a different technique is used, where the % hook remains in the body, and when macro is to be expanded the body is % processed again to replace the arguments. % % In that case, the hook is \the\toks N-1, and we simply set \toks N-1 to the % argument N value and then \edef the body (nothing else will expand because of % the catcode regime under which the body was input). % % If you compile with TeX (not eTeX), and you have macros with 10 or more % arguments, no macro can have more than 256 arguments (else error). % % In case that there are 10 or more arguments we parse again the arguments % list to set new definitions for the \macarg.BLAH macros corresponding to % each BLAH argument. It was anyhow needed to parse already once this list % in order to count the arguments, and as macros with at most 9 arguments % are by far more frequent than macro with 10 or more arguments, defining % twice the \macarg.BLAH macros does not cost too much processing power. \def\parsemmanyargdef@@#1,{% \if#1;\let\next=\relax \else \let\next=\parsemmanyargdef@@ \edef\tempb{\eatspaces{#1}}% \expandafter\def\expandafter\tempa \expandafter{\csname macarg.\tempb\endcsname}% % Note that we need some extra \noexpand\noexpand, this is because we % don't want \the to be expanded in the \parsermacbody as it uses an % \xdef . \expandafter\edef\tempa {\noexpand\noexpand\noexpand\the\toks\the\paramno}% \advance\paramno by 1\relax \fi\next} \let\endargs@\relax \let\nil@\relax \def\nilm@{\nil@}% \long\def\nillm@{\nil@}% % This macro is expanded during the Texinfo macro expansion, not during its % definition. It gets all the arguments' values and assigns them to macros % macarg.ARGNAME % % #1 is the macro name % #2 is the list of argument names % #3 is the list of argument values \def\getargvals@#1#2#3{% \def\macargdeflist@{}% \def\saveparamlist@{#2}% Need to keep a copy for parameter expansion. \def\paramlist{#2,\nil@}% \def\macroname{#1}% \begingroup \macroargctxt \def\argvaluelist{#3,\nil@}% \def\@tempa{#3}% \ifx\@tempa\empty \setemptyargvalues@ \else \getargvals@@ \fi } \def\getargvals@@{% \ifx\paramlist\nilm@ % Some sanity check needed here that \argvaluelist is also empty. \ifx\argvaluelist\nillm@ \else \errhelp = \EMsimple \errmessage{Too many arguments in macro `\macroname'!}% \fi \let\next\macargexpandinbody@ \else \ifx\argvaluelist\nillm@ % No more arguments values passed to macro. Set remaining named-arg % macros to empty. \let\next\setemptyargvalues@ \else % pop current arg name into \@tempb \def\@tempa##1{\pop@{\@tempb}{\paramlist}##1\endargs@}% \expandafter\@tempa\expandafter{\paramlist}% % pop current argument value into \@tempc \def\@tempa##1{\longpop@{\@tempc}{\argvaluelist}##1\endargs@}% \expandafter\@tempa\expandafter{\argvaluelist}% % Here \@tempb is the current arg name and \@tempc is the current arg value. % First place the new argument macro definition into \@tempd \expandafter\macname\expandafter{\@tempc}% \expandafter\let\csname macarg.\@tempb\endcsname\relax \expandafter\def\expandafter\@tempe\expandafter{% \csname macarg.\@tempb\endcsname}% \edef\@tempd{\long\def\@tempe{\the\macname}}% \push@\@tempd\macargdeflist@ \let\next\getargvals@@ \fi \fi \next } \def\push@#1#2{% \expandafter\expandafter\expandafter\def \expandafter\expandafter\expandafter#2% \expandafter\expandafter\expandafter{% \expandafter#1#2}% } % Replace arguments by their values in the macro body, and place the result % in macro \@tempa. % \def\macvalstoargs@{% % To do this we use the property that token registers that are \the'ed % within an \edef expand only once. So we are going to place all argument % values into respective token registers. % % First we save the token context, and initialize argument numbering. \begingroup \paramno0\relax % Then, for each argument number #N, we place the corresponding argument % value into a new token list register \toks#N \expandafter\putargsintokens@\saveparamlist@,;,% % Then, we expand the body so that argument are replaced by their % values. The trick for values not to be expanded themselves is that they % are within tokens and that tokens expand only once in an \edef . \edef\@tempc{\csname mac.\macroname .body\endcsname}% % Now we restore the token stack pointer to free the token list registers % which we have used, but we make sure that expanded body is saved after % group. \expandafter \endgroup \expandafter\def\expandafter\@tempa\expandafter{\@tempc}% } % Define the named-macro outside of this group and then close this group. % \def\macargexpandinbody@{% \expandafter \endgroup \macargdeflist@ % First the replace in body the macro arguments by their values, the result % is in \@tempa . \macvalstoargs@ % Then we point at the \norecurse or \gobble (for recursive) macro value % with \@tempb . \expandafter\let\expandafter\@tempb\csname mac.\macroname .recurse\endcsname % Depending on whether it is recursive or not, we need some tailing % \egroup . \ifx\@tempb\gobble \let\@tempc\relax \else \let\@tempc\egroup \fi % And now we do the real job: \edef\@tempd{\noexpand\@tempb{\macroname}\noexpand\scanmacro{\@tempa}\@tempc}% \@tempd } \def\putargsintokens@#1,{% \if#1;\let\next\relax \else \let\next\putargsintokens@ % First we allocate the new token list register, and give it a temporary % alias \@tempb . \toksdef\@tempb\the\paramno % Then we place the argument value into that token list register. \expandafter\let\expandafter\@tempa\csname macarg.#1\endcsname \expandafter\@tempb\expandafter{\@tempa}% \advance\paramno by 1\relax \fi \next } % Trailing missing arguments are set to empty. % \def\setemptyargvalues@{% \ifx\paramlist\nilm@ \let\next\macargexpandinbody@ \else \expandafter\setemptyargvaluesparser@\paramlist\endargs@ \let\next\setemptyargvalues@ \fi \next } \def\setemptyargvaluesparser@#1,#2\endargs@{% \expandafter\def\expandafter\@tempa\expandafter{% \expandafter\def\csname macarg.#1\endcsname{}}% \push@\@tempa\macargdeflist@ \def\paramlist{#2}% } % #1 is the element target macro % #2 is the list macro % #3,#4\endargs@ is the list value \def\pop@#1#2#3,#4\endargs@{% \def#1{#3}% \def#2{#4}% } \long\def\longpop@#1#2#3,#4\endargs@{% \long\def#1{#3}% \long\def#2{#4}% } %%%%%%%%%%%%%% End of code for > 10 arguments %%%%%%%%%%%%%%%%%% % This defines a Texinfo @macro or @rmacro, called by \parsemacbody. % \macrobody has the body of the macro in it, with placeholders for % its parameters, looking like "\xeatspaces{\hash 1}". % \paramno is the number of parameters % \paramlist is a TeX parameter text, e.g. "#1,#2,#3," % There are four cases: macros of zero, one, up to nine, and many arguments. % \xdef is used so that macro definitions will survive the file % they're defined in: @include reads the file inside a group. % \def\defmacro{% \let\hash=##% convert placeholders to macro parameter chars \ifnum\paramno=1 \def\xeatspaces##1{##1}% % This removes the pair of braces around the argument. We don't % use \eatspaces, because this can cause ends of lines to be lost % when the argument to \eatspaces is read, leading to line-based % commands like "@itemize" not being read correctly. \else \let\xeatspaces\relax % suppress expansion \fi \ifcase\paramno % 0 \expandafter\xdef\csname\the\macname\endcsname{% \bgroup \noexpand\spaceisspace \noexpand\endlineisspace \noexpand\expandafter % skip any whitespace after the macro name. \expandafter\noexpand\csname\the\macname @@@\endcsname}% \expandafter\xdef\csname\the\macname @@@\endcsname{% \egroup \noexpand\scanmacro{\macrobody}}% \or % 1 \expandafter\xdef\csname\the\macname\endcsname{% \bgroup \noexpand\braceorline \expandafter\noexpand\csname\the\macname @@@\endcsname}% \expandafter\xdef\csname\the\macname @@@\endcsname##1{% \egroup \noexpand\scanmacro{\macrobody}% }% \else % at most 9 \ifnum\paramno<10\relax % @MACNAME sets the context for reading the macro argument % @MACNAME@@ gets the argument, processes backslashes and appends a % comma. % @MACNAME@@@ removes braces surrounding the argument list. % @MACNAME@@@@ scans the macro body with arguments substituted. \expandafter\xdef\csname\the\macname\endcsname{% \bgroup \noexpand\expandafter % This \expandafter skip any spaces after the \noexpand\macroargctxt % macro before we change the catcode of space. \noexpand\expandafter \expandafter\noexpand\csname\the\macname @@\endcsname}% \expandafter\xdef\csname\the\macname @@\endcsname##1{% \noexpand\passargtomacro \expandafter\noexpand\csname\the\macname @@@\endcsname{##1,}}% \expandafter\xdef\csname\the\macname @@@\endcsname##1{% \expandafter\noexpand\csname\the\macname @@@@\endcsname ##1}% \expandafter\expandafter \expandafter\xdef \expandafter\expandafter \csname\the\macname @@@@\endcsname\paramlist{% \egroup\noexpand\scanmacro{\macrobody}}% \else % 10 or more: \expandafter\xdef\csname\the\macname\endcsname{% \noexpand\getargvals@{\the\macname}{\argl}% }% \global\expandafter\let\csname mac.\the\macname .body\endcsname\macrobody \global\expandafter\let\csname mac.\the\macname .recurse\endcsname\gobble \fi \fi} \catcode `\@\texiatcatcode\relax % end private-to-Texinfo catcodes \def\norecurse#1{\bgroup\cslet{#1}{macsave.#1}} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % {\catcode`\@=0 \catcode`\\=13 % We need to manipulate \ so use @ as escape @catcode`@_=11 % private names @catcode`@!=11 % used as argument separator % \passargtomacro#1#2 - % Call #1 with a list of tokens #2, with any doubled backslashes in #2 % compressed to one. % % This implementation works by expansion, and not execution (so we cannot use % \def or similar). This reduces the risk of this failing in contexts where % complete expansion is done with no execution (for example, in writing out to % an auxiliary file for an index entry). % % State is kept in the input stream: the argument passed to % @look_ahead, @gobble_and_check_finish and @add_segment is % % THE_MACRO ARG_RESULT ! {PENDING_BS} NEXT_TOKEN (... rest of input) % % where: % THE_MACRO - name of the macro we want to call % ARG_RESULT - argument list we build to pass to that macro % PENDING_BS - either a backslash or nothing % NEXT_TOKEN - used to look ahead in the input stream to see what's coming next @gdef@passargtomacro#1#2{% @add_segment #1!{}@relax#2\@_finish\% } @gdef@_finish{@_finishx} @global@let@_finishx@relax % #1 - THE_MACRO ARG_RESULT % #2 - PENDING_BS % #3 - NEXT_TOKEN % #4 used to look ahead % % If the next token is not a backslash, process the rest of the argument; % otherwise, remove the next token. @gdef@look_ahead#1!#2#3#4{% @ifx#4\% @expandafter@gobble_and_check_finish @else @expandafter@add_segment @fi#1!{#2}#4#4% } % #1 - THE_MACRO ARG_RESULT % #2 - PENDING_BS % #3 - NEXT_TOKEN % #4 should be a backslash, which is gobbled. % #5 looks ahead % % Double backslash found. Add a single backslash, and look ahead. @gdef@gobble_and_check_finish#1!#2#3#4#5{% @add_segment#1\!{}#5#5% } @gdef@is_fi{@fi} % #1 - THE_MACRO ARG_RESULT % #2 - PENDING_BS % #3 - NEXT_TOKEN % #4 is input stream until next backslash % % Input stream is either at the start of the argument, or just after a % backslash sequence, either a lone backslash, or a doubled backslash. % NEXT_TOKEN contains the first token in the input stream: if it is \finish, % finish; otherwise, append to ARG_RESULT the segment of the argument up until % the next backslash. PENDING_BACKSLASH contains a backslash to represent % a backslash just before the start of the input stream that has not been % added to ARG_RESULT. @gdef@add_segment#1!#2#3#4\{% @ifx#3@_finish @call_the_macro#1!% @else % append the pending backslash to the result, followed by the next segment @expandafter@is_fi@look_ahead#1#2#4!{\}@fi % this @fi is discarded by @look_ahead. % we can't get rid of it with \expandafter because we don't know how % long #4 is. } % #1 - THE_MACRO % #2 - ARG_RESULT % #3 discards the res of the conditional in @add_segment, and @is_fi ends the % conditional. @gdef@call_the_macro#1#2!#3@fi{@is_fi #1{#2}} } %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % \braceorline MAC is used for a one-argument macro MAC. It checks % whether the next non-whitespace character is a {. It sets the context % for reading the argument (slightly different in the two cases). Then, % to read the argument, in the whole-line case, it then calls the regular % \parsearg MAC; in the lbrace case, it calls \passargtomacro MAC. % \def\braceorline#1{\let\macnamexxx=#1\futurelet\nchar\braceorlinexxx} \def\braceorlinexxx{% \ifx\nchar\bgroup \macroargctxt \expandafter\passargtomacro \else \macrolineargctxt\expandafter\parsearg \fi \macnamexxx} % @alias. % We need some trickery to remove the optional spaces around the equal % sign. Make them active and then expand them all to nothing. % \def\alias{\parseargusing\obeyspaces\aliasxxx} \def\aliasxxx #1{\aliasyyy#1\relax} \def\aliasyyy #1=#2\relax{% {% \expandafter\let\obeyedspace=\empty \addtomacrolist{#1}% \xdef\next{\global\let\makecsname{#1}=\makecsname{#2}}% }% \next } \message{cross references,} \newwrite\auxfile \newif\ifhavexrefs % True if xref values are known. \newif\ifwarnedxrefs % True if we warned once that they aren't known. % @inforef is relatively simple. \def\inforef #1{\inforefzzz #1,,,,**} \def\inforefzzz #1,#2,#3,#4**{% \putwordSee{} \putwordInfo{} \putwordfile{} \file{\ignorespaces #3{}}, node \samp{\ignorespaces#1{}}} % @node's only job in TeX is to define \lastnode, which is used in % cross-references. The @node line might or might not have commas, and % might or might not have spaces before the first comma, like: % @node foo , bar , ... % We don't want such trailing spaces in the node name. % \parseargdef\node{\checkenv{}\donode #1 ,\finishnodeparse} % % also remove a trailing comma, in case of something like this: % @node Help-Cross, , , Cross-refs \def\donode#1 ,#2\finishnodeparse{\dodonode #1,\finishnodeparse} \def\dodonode#1,#2\finishnodeparse{\gdef\lastnode{#1}} \let\nwnode=\node \let\lastnode=\empty % Write a cross-reference definition for the current node. #1 is the % type (Ynumbered, Yappendix, Ynothing). % \def\donoderef#1{% \ifx\lastnode\empty\else \setref{\lastnode}{#1}% \global\let\lastnode=\empty \fi } % @anchor{NAME} -- define xref target at arbitrary point. % \newcount\savesfregister % \def\savesf{\relax \ifhmode \savesfregister=\spacefactor \fi} \def\restoresf{\relax \ifhmode \spacefactor=\savesfregister \fi} \def\anchor#1{\savesf \setref{#1}{Ynothing}\restoresf \ignorespaces} % \setref{NAME}{SNT} defines a cross-reference point NAME (a node or an % anchor), which consists of three parts: % 1) NAME-title - the current sectioning name taken from \lastsection, % or the anchor name. % 2) NAME-snt - section number and type, passed as the SNT arg, or % empty for anchors. % 3) NAME-pg - the page number. % % This is called from \donoderef, \anchor, and \dofloat. In the case of % floats, there is an additional part, which is not written here: % 4) NAME-lof - the text as it should appear in a @listoffloats. % \def\setref#1#2{% \pdfmkdest{#1}% \iflinks {% \requireauxfile \atdummies % preserve commands, but don't expand them % match definition in \xrdef, \refx, \xrefX. \def\value##1{##1}% \edef\writexrdef##1##2{% \write\auxfile{@xrdef{#1-% #1 of \setref, expanded by the \edef ##1}{##2}}% these are parameters of \writexrdef }% \toks0 = \expandafter{\lastsection}% \immediate \writexrdef{title}{\the\toks0 }% \immediate \writexrdef{snt}{\csname #2\endcsname}% \Ynumbered etc. \safewhatsit{\writexrdef{pg}{\folio}}% will be written later, at \shipout }% \fi } % @xrefautosectiontitle on|off says whether @section(ing) names are used % automatically in xrefs, if the third arg is not explicitly specified. % This was provided as a "secret" @set xref-automatic-section-title % variable, now it's official. % \parseargdef\xrefautomaticsectiontitle{% \def\temp{#1}% \ifx\temp\onword \expandafter\let\csname SETxref-automatic-section-title\endcsname = \empty \else\ifx\temp\offword \expandafter\let\csname SETxref-automatic-section-title\endcsname = \relax \else \errhelp = \EMsimple \errmessage{Unknown @xrefautomaticsectiontitle value `\temp', must be on|off}% \fi\fi } % % @xref, @pxref, and @ref generate cross-references. For \xrefX, #1 is % the node name, #2 the name of the Info cross-reference, #3 the printed % node name, #4 the name of the Info file, #5 the name of the printed % manual. All but the node name can be omitted. % \def\pxref{\putwordsee{} \xrefXX} \def\xref{\putwordSee{} \xrefXX} \def\ref{\xrefXX} \def\xrefXX#1{\def\xrefXXarg{#1}\futurelet\tokenafterxref\xrefXXX} \def\xrefXXX{\expandafter\xrefX\expandafter[\xrefXXarg,,,,,,,]} % \newbox\toprefbox \newbox\printedrefnamebox \newbox\infofilenamebox \newbox\printedmanualbox % \def\xrefX[#1,#2,#3,#4,#5,#6]{\begingroup \unsepspaces % % Get args without leading/trailing spaces. \def\printedrefname{\ignorespaces #3}% \setbox\printedrefnamebox = \hbox{\printedrefname\unskip}% % \def\infofilename{\ignorespaces #4}% \setbox\infofilenamebox = \hbox{\infofilename\unskip}% % \def\printedmanual{\ignorespaces #5}% \setbox\printedmanualbox = \hbox{\printedmanual\unskip}% % % If the printed reference name (arg #3) was not explicitly given in % the @xref, figure out what we want to use. \ifdim \wd\printedrefnamebox = 0pt % No printed node name was explicitly given. \expandafter\ifx\csname SETxref-automatic-section-title\endcsname \relax % Not auto section-title: use node name inside the square brackets. \def\printedrefname{\ignorespaces #1}% \else % Auto section-title: use chapter/section title inside % the square brackets if we have it. \ifdim \wd\printedmanualbox > 0pt % It is in another manual, so we don't have it; use node name. \def\printedrefname{\ignorespaces #1}% \else \ifhavexrefs % We (should) know the real title if we have the xref values. \def\printedrefname{\refx{#1-title}{}}% \else % Otherwise just copy the Info node name. \def\printedrefname{\ignorespaces #1}% \fi% \fi \fi \fi % % Make link in pdf output. \ifpdf % For pdfTeX and LuaTeX {\indexnofonts \makevalueexpandable \turnoffactive % This expands tokens, so do it after making catcode changes, so _ % etc. don't get their TeX definitions. This ignores all spaces in % #4, including (wrongly) those in the middle of the filename. \getfilename{#4}% % % This (wrongly) does not take account of leading or trailing % spaces in #1, which should be ignored. \setpdfdestname{#1}% % \ifx\pdfdestname\empty \def\pdfdestname{Top}% no empty targets \fi % \leavevmode \startlink attr{/Border [0 0 0]}% \ifnum\filenamelength>0 goto file{\the\filename.pdf} name{\pdfdestname}% \else goto name{\pdfmkpgn{\pdfdestname}}% \fi }% \setcolor{\linkcolor}% \else \ifx\XeTeXrevision\thisisundefined \else % For XeTeX {\indexnofonts \makevalueexpandable \turnoffactive % This expands tokens, so do it after making catcode changes, so _ % etc. don't get their TeX definitions. This ignores all spaces in % #4, including (wrongly) those in the middle of the filename. \getfilename{#4}% % % This (wrongly) does not take account of leading or trailing % spaces in #1, which should be ignored. \setpdfdestname{#1}% % \ifx\pdfdestname\empty \def\pdfdestname{Top}% no empty targets \fi % \leavevmode \ifnum\filenamelength>0 % With default settings, % XeTeX (xdvipdfmx) replaces link destination names with integers. % In this case, the replaced destination names of % remote PDFs are no longer known. In order to avoid a replacement, % you can use xdvipdfmx's command line option `-C 0x0010'. % If you use XeTeX 0.99996+ (TeX Live 2016+), % this command line option is no longer necessary % because we can use the `dvipdfmx:config' special. \special{pdf:bann << /Border [0 0 0] /Type /Annot /Subtype /Link /A << /S /GoToR /F (\the\filename.pdf) /D (\pdfdestname) >> >>}% \else \special{pdf:bann << /Border [0 0 0] /Type /Annot /Subtype /Link /A << /S /GoTo /D (\pdfdestname) >> >>}% \fi }% \setcolor{\linkcolor}% \fi \fi {% % Have to otherify everything special to allow the \csname to % include an _ in the xref name, etc. \indexnofonts \turnoffactive \def\value##1{##1}% \expandafter\global\expandafter\let\expandafter\Xthisreftitle \csname XR#1-title\endcsname }% % % Float references are printed completely differently: "Figure 1.2" % instead of "[somenode], p.3". \iffloat distinguishes them by % \Xthisreftitle being set to a magic string. \iffloat\Xthisreftitle % If the user specified the print name (third arg) to the ref, % print it instead of our usual "Figure 1.2". \ifdim\wd\printedrefnamebox = 0pt \refx{#1-snt}{}% \else \printedrefname \fi % % If the user also gave the printed manual name (fifth arg), append % "in MANUALNAME". \ifdim \wd\printedmanualbox > 0pt \space \putwordin{} \cite{\printedmanual}% \fi \else % node/anchor (non-float) references. % % If we use \unhbox to print the node names, TeX does not insert % empty discretionaries after hyphens, which means that it will not % find a line break at a hyphen in a node names. Since some manuals % are best written with fairly long node names, containing hyphens, % this is a loss. Therefore, we give the text of the node name % again, so it is as if TeX is seeing it for the first time. % \ifdim \wd\printedmanualbox > 0pt % Cross-manual reference with a printed manual name. % \crossmanualxref{\cite{\printedmanual\unskip}}% % \else\ifdim \wd\infofilenamebox > 0pt % Cross-manual reference with only an info filename (arg 4), no % printed manual name (arg 5). This is essentially the same as % the case above; we output the filename, since we have nothing else. % \crossmanualxref{\code{\infofilename\unskip}}% % \else % Reference within this manual. % % _ (for example) has to be the character _ for the purposes of the % control sequence corresponding to the node, but it has to expand % into the usual \leavevmode...\vrule stuff for purposes of % printing. So we \turnoffactive for the \refx-snt, back on for the % printing, back off for the \refx-pg. {\turnoffactive % Only output a following space if the -snt ref is nonempty; for % @unnumbered and @anchor, it won't be. \setbox2 = \hbox{\ignorespaces \refx{#1-snt}{}}% \ifdim \wd2 > 0pt \refx{#1-snt}\space\fi }% % output the `[mynode]' via the macro below so it can be overridden. \xrefprintnodename\printedrefname % % But we always want a comma and a space: ,\space % % output the `page 3'. \turnoffactive \putwordpage\tie\refx{#1-pg}{}% % Add a , if xref followed by a space \if\space\noexpand\tokenafterxref ,% \else\ifx\ \tokenafterxref ,% @TAB \else\ifx\*\tokenafterxref ,% @* \else\ifx\ \tokenafterxref ,% @SPACE \else\ifx\ \tokenafterxref ,% @NL \else\ifx\tie\tokenafterxref ,% @tie \fi\fi\fi\fi\fi\fi \fi\fi \fi \endlink \endgroup} % Output a cross-manual xref to #1. Used just above (twice). % % Only include the text "Section ``foo'' in" if the foo is neither % missing or Top. Thus, @xref{,,,foo,The Foo Manual} outputs simply % "see The Foo Manual", the idea being to refer to the whole manual. % % But, this being TeX, we can't easily compare our node name against the % string "Top" while ignoring the possible spaces before and after in % the input. By adding the arbitrary 7sp below, we make it much less % likely that a real node name would have the same width as "Top" (e.g., % in a monospaced font). Hopefully it will never happen in practice. % % For the same basic reason, we retypeset the "Top" at every % reference, since the current font is indeterminate. % \def\crossmanualxref#1{% \setbox\toprefbox = \hbox{Top\kern7sp}% \setbox2 = \hbox{\ignorespaces \printedrefname \unskip \kern7sp}% \ifdim \wd2 > 7sp % nonempty? \ifdim \wd2 = \wd\toprefbox \else % same as Top? \putwordSection{} ``\printedrefname'' \putwordin{}\space \fi \fi #1% } % This macro is called from \xrefX for the `[nodename]' part of xref % output. It's a separate macro only so it can be changed more easily, % since square brackets don't work well in some documents. Particularly % one that Bob is working on :). % \def\xrefprintnodename#1{[#1]} % Things referred to by \setref. % \def\Ynothing{} \def\Yomitfromtoc{} \def\Ynumbered{% \ifnum\secno=0 \putwordChapter@tie \the\chapno \else \ifnum\subsecno=0 \putwordSection@tie \the\chapno.\the\secno \else \ifnum\subsubsecno=0 \putwordSection@tie \the\chapno.\the\secno.\the\subsecno \else \putwordSection@tie \the\chapno.\the\secno.\the\subsecno.\the\subsubsecno \fi\fi\fi } \def\Yappendix{% \ifnum\secno=0 \putwordAppendix@tie @char\the\appendixno{}% \else \ifnum\subsecno=0 \putwordSection@tie @char\the\appendixno.\the\secno \else \ifnum\subsubsecno=0 \putwordSection@tie @char\the\appendixno.\the\secno.\the\subsecno \else \putwordSection@tie @char\the\appendixno.\the\secno.\the\subsecno.\the\subsubsecno \fi\fi\fi } % \refx{NAME}{SUFFIX} - reference a cross-reference string named NAME. SUFFIX % is output afterwards if non-empty. \def\refx#1#2{% \requireauxfile {% \indexnofonts \otherbackslash \def\value##1{##1}% \expandafter\global\expandafter\let\expandafter\thisrefX \csname XR#1\endcsname }% \ifx\thisrefX\relax % If not defined, say something at least. \angleleft un\-de\-fined\angleright \iflinks \ifhavexrefs {\toks0 = {#1}% avoid expansion of possibly-complex value \message{\linenumber Undefined cross reference `\the\toks0'.}}% \else \ifwarnedxrefs\else \global\warnedxrefstrue \message{Cross reference values unknown; you must run TeX again.}% \fi \fi \fi \else % It's defined, so just use it. \thisrefX \fi #2% Output the suffix in any case. } % This is the macro invoked by entries in the aux file. Define a control % sequence for a cross-reference target (we prepend XR to the control sequence % name to avoid collisions). The value is the page number. If this is a float % type, we have more work to do. % \def\xrdef#1#2{% {% Expand the node or anchor name to remove control sequences. % \turnoffactive stops 8-bit characters being changed to commands % like @'e. \refx does the same to retrieve the value in the definition. \indexnofonts \turnoffactive \def\value##1{##1}% \xdef\safexrefname{#1}% }% % \bgroup \expandafter\gdef\csname XR\safexrefname\endcsname{#2}% \egroup % We put the \gdef inside a group to avoid the definitions building up on % TeX's save stack, which can cause it to run out of space for aux files with % thousands of lines. \gdef doesn't use the save stack, but \csname does % when it defines an unknown control sequence as \relax. % % Was that xref control sequence that we just defined for a float? \expandafter\iffloat\csname XR\safexrefname\endcsname % it was a float, and we have the (safe) float type in \iffloattype. \expandafter\let\expandafter\floatlist \csname floatlist\iffloattype\endcsname % % Is this the first time we've seen this float type? \expandafter\ifx\floatlist\relax \toks0 = {\do}% yes, so just \do \else % had it before, so preserve previous elements in list. \toks0 = \expandafter{\floatlist\do}% \fi % % Remember this xref in the control sequence \floatlistFLOATTYPE, % for later use in \listoffloats. \expandafter\xdef\csname floatlist\iffloattype\endcsname{\the\toks0 {\safexrefname}}% \fi } % If working on a large document in chapters, it is convenient to % be able to disable indexing, cross-referencing, and contents, for test runs. % This is done with @novalidate at the beginning of the file. % \newif\iflinks \linkstrue % by default we want the aux files. \let\novalidate = \linksfalse % Used when writing to the aux file, or when using data from it. \def\requireauxfile{% \iflinks \tryauxfile % Open the new aux file. TeX will close it automatically at exit. \immediate\openout\auxfile=\jobname.aux \fi \global\let\requireauxfile=\relax % Only do this once. } % Read the last existing aux file, if any. No error if none exists. % \def\tryauxfile{% \openin 1 \jobname.aux \ifeof 1 \else \readdatafile{aux}% \global\havexrefstrue \fi \closein 1 } \def\setupdatafile{% \catcode`\^^@=\other \catcode`\^^A=\other \catcode`\^^B=\other \catcode`\^^C=\other \catcode`\^^D=\other \catcode`\^^E=\other \catcode`\^^F=\other \catcode`\^^G=\other \catcode`\^^H=\other \catcode`\^^K=\other \catcode`\^^L=\other \catcode`\^^N=\other \catcode`\^^P=\other \catcode`\^^Q=\other \catcode`\^^R=\other \catcode`\^^S=\other \catcode`\^^T=\other \catcode`\^^U=\other \catcode`\^^V=\other \catcode`\^^W=\other \catcode`\^^X=\other \catcode`\^^Z=\other \catcode`\^^[=\other \catcode`\^^\=\other \catcode`\^^]=\other \catcode`\^^^=\other \catcode`\^^_=\other % It was suggested to set the catcode of ^ to 7, which would allow ^^e4 etc. % in xref tags, i.e., node names. But since ^^e4 notation isn't % supported in the main text, it doesn't seem desirable. Furthermore, % that is not enough: for node names that actually contain a ^ % character, we would end up writing a line like this: 'xrdef {'hat % b-title}{'hat b} and \xrdef does a \csname...\endcsname on the first % argument, and \hat is not an expandable control sequence. It could % all be worked out, but why? Either we support ^^ or we don't. % % The other change necessary for this was to define \auxhat: % \def\auxhat{\def^{'hat }}% extra space so ok if followed by letter % and then to call \auxhat in \setq. % \catcode`\^=\other % % Special characters. Should be turned off anyway, but... \catcode`\~=\other \catcode`\[=\other \catcode`\]=\other \catcode`\"=\other \catcode`\_=\other \catcode`\|=\other \catcode`\<=\other \catcode`\>=\other \catcode`\$=\other \catcode`\#=\other \catcode`\&=\other \catcode`\%=\other \catcode`+=\other % avoid \+ for paranoia even though we've turned it off % % This is to support \ in node names and titles, since the \ % characters end up in a \csname. It's easier than % leaving it active and making its active definition an actual \ % character. What I don't understand is why it works in the *value* % of the xrdef. Seems like it should be a catcode12 \, and that % should not typeset properly. But it works, so I'm moving on for % now. --karl, 15jan04. \catcode`\\=\other % % @ is our escape character in .aux files, and we need braces. \catcode`\{=1 \catcode`\}=2 \catcode`\@=0 } \def\readdatafile#1{% \begingroup \setupdatafile \input\jobname.#1 \endgroup} \message{insertions,} % including footnotes. \newcount \footnoteno % The trailing space in the following definition for supereject is % vital for proper filling; pages come out unaligned when you do a % pagealignmacro call if that space before the closing brace is % removed. (Generally, numeric constants should always be followed by a % space to prevent strange expansion errors.) \def\supereject{\par\penalty -20000\footnoteno =0 } % @footnotestyle is meaningful for Info output only. \let\footnotestyle=\comment {\catcode `\@=11 % % Auto-number footnotes. Otherwise like plain. \gdef\footnote{% \global\advance\footnoteno by \@ne \edef\thisfootno{$^{\the\footnoteno}$}% % % In case the footnote comes at the end of a sentence, preserve the % extra spacing after we do the footnote number. \let\@sf\empty \ifhmode\edef\@sf{\spacefactor\the\spacefactor}\ptexslash\fi % % Remove inadvertent blank space before typesetting the footnote number. \unskip \thisfootno\@sf \dofootnote }% % Don't bother with the trickery in plain.tex to not require the % footnote text as a parameter. Our footnotes don't need to be so general. % % Oh yes, they do; otherwise, @ifset (and anything else that uses % \parseargline) fails inside footnotes because the tokens are fixed when % the footnote is read. --karl, 16nov96. % \gdef\dofootnote{% \insert\footins\bgroup % % Nested footnotes are not supported in TeX, that would take a lot % more work. (\startsavinginserts does not suffice.) \let\footnote=\errfootnotenest % % We want to typeset this text as a normal paragraph, even if the % footnote reference occurs in (for example) a display environment. % So reset some parameters. \hsize=\txipagewidth \interlinepenalty\interfootnotelinepenalty \splittopskip\ht\strutbox % top baseline for broken footnotes \splitmaxdepth\dp\strutbox \floatingpenalty\@MM \leftskip\z@skip \rightskip\z@skip \spaceskip\z@skip \xspaceskip\z@skip \parindent\defaultparindent % \smallfonts \rm % % Because we use hanging indentation in footnotes, a @noindent appears % to exdent this text, so make it be a no-op. makeinfo does not use % hanging indentation so @noindent can still be needed within footnote % text after an @example or the like (not that this is good style). \let\noindent = \relax % % Hang the footnote text off the number. Use \everypar in case the % footnote extends for more than one paragraph. \everypar = {\hang}% \textindent{\thisfootno}% % % Don't crash into the line above the footnote text. Since this % expands into a box, it must come within the paragraph, lest it % provide a place where TeX can split the footnote. \footstrut % % Invoke rest of plain TeX footnote routine. \futurelet\next\fo@t } }%end \catcode `\@=11 \def\errfootnotenest{% \errhelp=\EMsimple \errmessage{Nested footnotes not supported in texinfo.tex, even though they work in makeinfo; sorry} } \def\errfootnoteheading{% \errhelp=\EMsimple \errmessage{Footnotes in chapters, sections, etc., are not supported} } % In case a @footnote appears in a vbox, save the footnote text and create % the real \insert just after the vbox finished. Otherwise, the insertion % would be lost. % Similarly, if a @footnote appears inside an alignment, save the footnote % text to a box and make the \insert when a row of the table is finished. % And the same can be done for other insert classes. --kasal, 16nov03. % % Replace the \insert primitive by a cheating macro. % Deeper inside, just make sure that the saved insertions are not spilled % out prematurely. % \def\startsavinginserts{% \ifx \insert\ptexinsert \let\insert\saveinsert \else \let\checkinserts\relax \fi } % This \insert replacement works for both \insert\footins{foo} and % \insert\footins\bgroup foo\egroup, but it doesn't work for \insert27{foo}. % \def\saveinsert#1{% \edef\next{\noexpand\savetobox \makeSAVEname#1}% \afterassignment\next % swallow the left brace \let\temp = } \def\makeSAVEname#1{\makecsname{SAVE\expandafter\gobble\string#1}} \def\savetobox#1{\global\setbox#1 = \vbox\bgroup \unvbox#1} \def\checksaveins#1{\ifvoid#1\else \placesaveins#1\fi} \def\placesaveins#1{% \ptexinsert \csname\expandafter\gobblesave\string#1\endcsname {\box#1}% } % eat @SAVE -- beware, all of them have catcode \other: { \def\dospecials{\do S\do A\do V\do E} \uncatcodespecials % ;-) \gdef\gobblesave @SAVE{} } % initialization: \def\newsaveins #1{% \edef\next{\noexpand\newsaveinsX \makeSAVEname#1}% \next } \def\newsaveinsX #1{% \csname newbox\endcsname #1% \expandafter\def\expandafter\checkinserts\expandafter{\checkinserts \checksaveins #1}% } % initialize: \let\checkinserts\empty \newsaveins\footins \newsaveins\margin % @image. We use the macros from epsf.tex to support this. % If epsf.tex is not installed and @image is used, we complain. % % Check for and read epsf.tex up front. If we read it only at @image % time, we might be inside a group, and then its definitions would get % undone and the next image would fail. \openin 1 = epsf.tex \ifeof 1 \else % Do not bother showing banner with epsf.tex v2.7k (available in % doc/epsf.tex and on ctan). \def\epsfannounce{\toks0 = }% \input epsf.tex \fi \closein 1 % % We will only complain once about lack of epsf.tex. \newif\ifwarnednoepsf \newhelp\noepsfhelp{epsf.tex must be installed for images to work. It is also included in the Texinfo distribution, or you can get it from https://ctan.org/texarchive/macros/texinfo/texinfo/doc/epsf.tex.} % \def\image#1{% \ifx\epsfbox\thisisundefined \ifwarnednoepsf \else \errhelp = \noepsfhelp \errmessage{epsf.tex not found, images will be ignored}% \global\warnednoepsftrue \fi \else \imagexxx #1,,,,,\finish \fi } % % Arguments to @image: % #1 is (mandatory) image filename; we tack on .eps extension. % #2 is (optional) width, #3 is (optional) height. % #4 is (ignored optional) html alt text. % #5 is (ignored optional) extension. % #6 is just the usual extra ignored arg for parsing stuff. \newif\ifimagevmode \def\imagexxx#1,#2,#3,#4,#5,#6\finish{\begingroup \catcode`\^^M = 5 % in case we're inside an example \normalturnoffactive % allow _ et al. in names \def\xprocessmacroarg{\eatspaces}% in case we are being used via a macro % If the image is by itself, center it. \ifvmode \imagevmodetrue \else \ifx\centersub\centerV % for @center @image, we need a vbox so we can have our vertical space \imagevmodetrue \vbox\bgroup % vbox has better behavior than vtop herev \fi\fi % \ifimagevmode \nobreak\medskip % Usually we'll have text after the image which will insert % \parskip glue, so insert it here too to equalize the space % above and below. \nobreak\vskip\parskip \nobreak \fi % % Leave vertical mode so that indentation from an enclosing % environment such as @quotation is respected. % However, if we're at the top level, we don't want the % normal paragraph indentation. % On the other hand, if we are in the case of @center @image, we don't % want to start a paragraph, which will create a hsize-width box and % eradicate the centering. \ifx\centersub\centerV\else \noindent \fi % % Output the image. \ifpdf % For pdfTeX and LuaTeX <= 0.80 \dopdfimage{#1}{#2}{#3}% \else \ifx\XeTeXrevision\thisisundefined % For epsf.tex % \epsfbox itself resets \epsf?size at each figure. \setbox0 = \hbox{\ignorespaces #2}% \ifdim\wd0 > 0pt \epsfxsize=#2\relax \fi \setbox0 = \hbox{\ignorespaces #3}% \ifdim\wd0 > 0pt \epsfysize=#3\relax \fi \epsfbox{#1.eps}% \else % For XeTeX \doxeteximage{#1}{#2}{#3}% \fi \fi % \ifimagevmode \medskip % space after a standalone image \fi \ifx\centersub\centerV \egroup \fi \endgroup} % @float FLOATTYPE,LABEL,LOC ... @end float for displayed figures, tables, % etc. We don't actually implement floating yet, we always include the % float "here". But it seemed the best name for the future. % \envparseargdef\float{\eatcommaspace\eatcommaspace\dofloat#1, , ,\finish} % There may be a space before second and/or third parameter; delete it. \def\eatcommaspace#1, {#1,} % #1 is the optional FLOATTYPE, the text label for this float, typically % "Figure", "Table", "Example", etc. Can't contain commas. If omitted, % this float will not be numbered and cannot be referred to. % % #2 is the optional xref label. Also must be present for the float to % be referable. % % #3 is the optional positioning argument; for now, it is ignored. It % will somehow specify the positions allowed to float to (here, top, bottom). % % We keep a separate counter for each FLOATTYPE, which we reset at each % chapter-level command. \let\resetallfloatnos=\empty % \def\dofloat#1,#2,#3,#4\finish{% \let\thiscaption=\empty \let\thisshortcaption=\empty % % don't lose footnotes inside @float. % % BEWARE: when the floats start float, we have to issue warning whenever an % insert appears inside a float which could possibly float. --kasal, 26may04 % \startsavinginserts % % We can't be used inside a paragraph. \par % \vtop\bgroup \def\floattype{#1}% \def\floatlabel{#2}% \def\floatloc{#3}% we do nothing with this yet. % \ifx\floattype\empty \let\safefloattype=\empty \else {% % the floattype might have accents or other special characters, % but we need to use it in a control sequence name. \indexnofonts \turnoffactive \xdef\safefloattype{\floattype}% }% \fi % % If label is given but no type, we handle that as the empty type. \ifx\floatlabel\empty \else % We want each FLOATTYPE to be numbered separately (Figure 1, % Table 1, Figure 2, ...). (And if no label, no number.) % \expandafter\getfloatno\csname\safefloattype floatno\endcsname \global\advance\floatno by 1 % {% % This magic value for \lastsection is output by \setref as the % XREFLABEL-title value. \xrefX uses it to distinguish float % labels (which have a completely different output format) from % node and anchor labels. And \xrdef uses it to construct the % lists of floats. % \edef\lastsection{\floatmagic=\safefloattype}% \setref{\floatlabel}{Yfloat}% }% \fi % % start with \parskip glue, I guess. \vskip\parskip % % Don't suppress indentation if a float happens to start a section. \restorefirstparagraphindent } % we have these possibilities: % @float Foo,lbl & @caption{Cap}: Foo 1.1: Cap % @float Foo,lbl & no caption: Foo 1.1 % @float Foo & @caption{Cap}: Foo: Cap % @float Foo & no caption: Foo % @float ,lbl & Caption{Cap}: 1.1: Cap % @float ,lbl & no caption: 1.1 % @float & @caption{Cap}: Cap % @float & no caption: % \def\Efloat{% \let\floatident = \empty % % In all cases, if we have a float type, it comes first. \ifx\floattype\empty \else \def\floatident{\floattype}\fi % % If we have an xref label, the number comes next. \ifx\floatlabel\empty \else \ifx\floattype\empty \else % if also had float type, need tie first. \appendtomacro\floatident{\tie}% \fi % the number. \appendtomacro\floatident{\chaplevelprefix\the\floatno}% \fi % % Start the printed caption with what we've constructed in % \floatident, but keep it separate; we need \floatident again. \let\captionline = \floatident % \ifx\thiscaption\empty \else \ifx\floatident\empty \else \appendtomacro\captionline{: }% had ident, so need a colon between \fi % % caption text. \appendtomacro\captionline{\scanexp\thiscaption}% \fi % % If we have anything to print, print it, with space before. % Eventually this needs to become an \insert. \ifx\captionline\empty \else \vskip.5\parskip \captionline % % Space below caption. \vskip\parskip \fi % % If have an xref label, write the list of floats info. Do this % after the caption, to avoid chance of it being a breakpoint. \ifx\floatlabel\empty \else % Write the text that goes in the lof to the aux file as % \floatlabel-lof. Besides \floatident, we include the short % caption if specified, else the full caption if specified, else nothing. {% \requireauxfile \atdummies % \ifx\thisshortcaption\empty \def\gtemp{\thiscaption}% \else \def\gtemp{\thisshortcaption}% \fi \immediate\write\auxfile{@xrdef{\floatlabel-lof}{\floatident \ifx\gtemp\empty \else : \gtemp \fi}}% }% \fi \egroup % end of \vtop % \checkinserts } % Append the tokens #2 to the definition of macro #1, not expanding either. % \def\appendtomacro#1#2{% \expandafter\def\expandafter#1\expandafter{#1#2}% } % @caption, @shortcaption % \def\caption{\docaption\thiscaption} \def\shortcaption{\docaption\thisshortcaption} \def\docaption{\checkenv\float \bgroup\scanargctxt\defcaption} \def\defcaption#1#2{\egroup \def#1{#2}} % The parameter is the control sequence identifying the counter we are % going to use. Create it if it doesn't exist and assign it to \floatno. \def\getfloatno#1{% \ifx#1\relax % Haven't seen this figure type before. \csname newcount\endcsname #1% % % Remember to reset this floatno at the next chap. \expandafter\gdef\expandafter\resetallfloatnos \expandafter{\resetallfloatnos #1=0 }% \fi \let\floatno#1% } % \setref calls this to get the XREFLABEL-snt value. We want an @xref % to the FLOATLABEL to expand to "Figure 3.1". We call \setref when we % first read the @float command. % \def\Yfloat{\floattype@tie \chaplevelprefix\the\floatno}% % Magic string used for the XREFLABEL-title value, so \xrefX can % distinguish floats from other xref types. \def\floatmagic{!!float!!} % #1 is the control sequence we are passed; we expand into a conditional % which is true if #1 represents a float ref. That is, the magic % \lastsection value which we \setref above. % \def\iffloat#1{\expandafter\doiffloat#1==\finish} % % #1 is (maybe) the \floatmagic string. If so, #2 will be the % (safe) float type for this float. We set \iffloattype to #2. % \def\doiffloat#1=#2=#3\finish{% \def\temp{#1}% \def\iffloattype{#2}% \ifx\temp\floatmagic } % @listoffloats FLOATTYPE - print a list of floats like a table of contents. % \parseargdef\listoffloats{% \def\floattype{#1}% floattype {% % the floattype might have accents or other special characters, % but we need to use it in a control sequence name. \indexnofonts \turnoffactive \xdef\safefloattype{\floattype}% }% % % \xrdef saves the floats as a \do-list in \floatlistSAFEFLOATTYPE. \expandafter\ifx\csname floatlist\safefloattype\endcsname \relax \ifhavexrefs % if the user said @listoffloats foo but never @float foo. \message{\linenumber No `\safefloattype' floats to list.}% \fi \else \begingroup \leftskip=\tocindent % indent these entries like a toc \let\do=\listoffloatsdo \csname floatlist\safefloattype\endcsname \endgroup \fi } % This is called on each entry in a list of floats. We're passed the % xref label, in the form LABEL-title, which is how we save it in the % aux file. We strip off the -title and look up \XRLABEL-lof, which % has the text we're supposed to typeset here. % % Figures without xref labels will not be included in the list (since % they won't appear in the aux file). % \def\listoffloatsdo#1{\listoffloatsdoentry#1\finish} \def\listoffloatsdoentry#1-title\finish{{% % Can't fully expand XR#1-lof because it can contain anything. Just % pass the control sequence. On the other hand, XR#1-pg is just the % page number, and we want to fully expand that so we can get a link % in pdf output. \toksA = \expandafter{\csname XR#1-lof\endcsname}% % % use the same \entry macro we use to generate the TOC and index. \edef\writeentry{\noexpand\entry{\the\toksA}{\csname XR#1-pg\endcsname}}% \writeentry }} \message{localization,} % For single-language documents, @documentlanguage is usually given very % early, just after @documentencoding. Single argument is the language % (de) or locale (de_DE) abbreviation. % { \catcode`\_ = \active \globaldefs=1 \parseargdef\documentlanguage{% \tex % read txi-??.tex file in plain TeX. % Read the file by the name they passed if it exists. \let_ = \normalunderscore % normal _ character for filename test \openin 1 txi-#1.tex \ifeof 1 \documentlanguagetrywithoutunderscore #1_\finish \else \globaldefs = 1 % everything in the txi-LL files needs to persist \input txi-#1.tex \fi \closein 1 \endgroup % end raw TeX } % % If they passed de_DE, and txi-de_DE.tex doesn't exist, % try txi-de.tex. % \gdef\documentlanguagetrywithoutunderscore#1_#2\finish{% \openin 1 txi-#1.tex \ifeof 1 \errhelp = \nolanghelp \errmessage{Cannot read language file txi-#1.tex}% \else \globaldefs = 1 % everything in the txi-LL files needs to persist \input txi-#1.tex \fi \closein 1 } }% end of special _ catcode % \newhelp\nolanghelp{The given language definition file cannot be found or is empty. Maybe you need to install it? Putting it in the current directory should work if nowhere else does.} % This macro is called from txi-??.tex files; the first argument is the % \language name to set (without the "\lang@" prefix), the second and % third args are \{left,right}hyphenmin. % % The language names to pass are determined when the format is built. % See the etex.log file created at that time, e.g., % /usr/local/texlive/2008/texmf-var/web2c/pdftex/etex.log. % % With TeX Live 2008, etex now includes hyphenation patterns for all % available languages. This means we can support hyphenation in % Texinfo, at least to some extent. (This still doesn't solve the % accented characters problem.) % \catcode`@=11 \def\txisetlanguage#1#2#3{% % do not set the language if the name is undefined in the current TeX. \expandafter\ifx\csname lang@#1\endcsname \relax \message{no patterns for #1}% \else \global\language = \csname lang@#1\endcsname \fi % but there is no harm in adjusting the hyphenmin values regardless. \global\lefthyphenmin = #2\relax \global\righthyphenmin = #3\relax } % XeTeX and LuaTeX can handle Unicode natively. % Their default I/O uses UTF-8 sequences instead of a byte-wise operation. % Other TeX engines' I/O (pdfTeX, etc.) is byte-wise. % \newif\iftxinativeunicodecapable \newif\iftxiusebytewiseio \ifx\XeTeXrevision\thisisundefined \ifx\luatexversion\thisisundefined \txinativeunicodecapablefalse \txiusebytewiseiotrue \else \txinativeunicodecapabletrue \txiusebytewiseiofalse \fi \else \txinativeunicodecapabletrue \txiusebytewiseiofalse \fi % Set I/O by bytes instead of UTF-8 sequence for XeTeX and LuaTex % for non-UTF-8 (byte-wise) encodings. % \def\setbytewiseio{% \ifx\XeTeXrevision\thisisundefined \else \XeTeXdefaultencoding "bytes" % For subsequent files to be read \XeTeXinputencoding "bytes" % For document root file % Unfortunately, there seems to be no corresponding XeTeX command for % output encoding. This is a problem for auxiliary index and TOC files. % The only solution would be perhaps to write out @U{...} sequences in % place of non-ASCII characters. \fi \ifx\luatexversion\thisisundefined \else \directlua{ local utf8_char, byte, gsub = unicode.utf8.char, string.byte, string.gsub local function convert_char (char) return utf8_char(byte(char)) end local function convert_line (line) return gsub(line, ".", convert_char) end callback.register("process_input_buffer", convert_line) local function convert_line_out (line) local line_out = "" for c in string.utfvalues(line) do line_out = line_out .. string.char(c) end return line_out end callback.register("process_output_buffer", convert_line_out) } \fi \txiusebytewiseiotrue } % Helpers for encodings. % Set the catcode of characters 128 through 255 to the specified number. % \def\setnonasciicharscatcode#1{% \count255=128 \loop\ifnum\count255<256 \global\catcode\count255=#1\relax \advance\count255 by 1 \repeat } \def\setnonasciicharscatcodenonglobal#1{% \count255=128 \loop\ifnum\count255<256 \catcode\count255=#1\relax \advance\count255 by 1 \repeat } % @documentencoding sets the definition of non-ASCII characters % according to the specified encoding. % \def\documentencoding{\parseargusing\filenamecatcodes\documentencodingzzz} \def\documentencodingzzz#1{% % % Encoding being declared for the document. \def\declaredencoding{\csname #1.enc\endcsname}% % % Supported encodings: names converted to tokens in order to be able % to compare them with \ifx. \def\ascii{\csname US-ASCII.enc\endcsname}% \def\latnine{\csname ISO-8859-15.enc\endcsname}% \def\latone{\csname ISO-8859-1.enc\endcsname}% \def\lattwo{\csname ISO-8859-2.enc\endcsname}% \def\utfeight{\csname UTF-8.enc\endcsname}% % \ifx \declaredencoding \ascii \asciichardefs % \else \ifx \declaredencoding \lattwo \iftxinativeunicodecapable \setbytewiseio \fi \setnonasciicharscatcode\active \lattwochardefs % \else \ifx \declaredencoding \latone \iftxinativeunicodecapable \setbytewiseio \fi \setnonasciicharscatcode\active \latonechardefs % \else \ifx \declaredencoding \latnine \iftxinativeunicodecapable \setbytewiseio \fi \setnonasciicharscatcode\active \latninechardefs % \else \ifx \declaredencoding \utfeight \iftxinativeunicodecapable % For native Unicode handling (XeTeX and LuaTeX) \nativeunicodechardefs \else % For treating UTF-8 as byte sequences (TeX, eTeX and pdfTeX) \setnonasciicharscatcode\active % since we already invoked \utfeightchardefs at the top level % (below), do not re-invoke it, otherwise our check for duplicated % definitions gets triggered. Making non-ascii chars active is % sufficient. \fi % \else \message{Ignoring unknown document encoding: #1.}% % \fi % utfeight \fi % latnine \fi % latone \fi % lattwo \fi % ascii % \ifx\XeTeXrevision\thisisundefined \else \ifx \declaredencoding \utfeight \else \ifx \declaredencoding \ascii \else \message{Warning: XeTeX with non-UTF-8 encodings cannot handle % non-ASCII characters in auxiliary files.}% \fi \fi \fi } % emacs-page % A message to be logged when using a character that isn't available % the default font encoding (OT1). % \def\missingcharmsg#1{\message{Character missing, sorry: #1.}} % Take account of \c (plain) vs. \, (Texinfo) difference. \def\cedilla#1{\ifx\c\ptexc\c{#1}\else\,{#1}\fi} % First, make active non-ASCII characters in order for them to be % correctly categorized when TeX reads the replacement text of % macros containing the character definitions. \setnonasciicharscatcode\active % \def\gdefchar#1#2{% \gdef#1{% \ifpassthroughchars \string#1% \else #2% \fi }} % Latin1 (ISO-8859-1) character definitions. \def\latonechardefs{% \gdefchar^^a0{\tie} \gdefchar^^a1{\exclamdown} \gdefchar^^a2{{\tcfont \char162}} % cent \gdefchar^^a3{\pounds{}} \gdefchar^^a4{{\tcfont \char164}} % currency \gdefchar^^a5{{\tcfont \char165}} % yen \gdefchar^^a6{{\tcfont \char166}} % broken bar \gdefchar^^a7{\S} \gdefchar^^a8{\"{}} \gdefchar^^a9{\copyright{}} \gdefchar^^aa{\ordf} \gdefchar^^ab{\guillemetleft{}} \gdefchar^^ac{\ensuremath\lnot} \gdefchar^^ad{\-} \gdefchar^^ae{\registeredsymbol{}} \gdefchar^^af{\={}} % \gdefchar^^b0{\textdegree} \gdefchar^^b1{$\pm$} \gdefchar^^b2{$^2$} \gdefchar^^b3{$^3$} \gdefchar^^b4{\'{}} \gdefchar^^b5{$\mu$} \gdefchar^^b6{\P} \gdefchar^^b7{\ensuremath\cdot} \gdefchar^^b8{\cedilla\ } \gdefchar^^b9{$^1$} \gdefchar^^ba{\ordm} \gdefchar^^bb{\guillemetright{}} \gdefchar^^bc{$1\over4$} \gdefchar^^bd{$1\over2$} \gdefchar^^be{$3\over4$} \gdefchar^^bf{\questiondown} % \gdefchar^^c0{\`A} \gdefchar^^c1{\'A} \gdefchar^^c2{\^A} \gdefchar^^c3{\~A} \gdefchar^^c4{\"A} \gdefchar^^c5{\ringaccent A} \gdefchar^^c6{\AE} \gdefchar^^c7{\cedilla C} \gdefchar^^c8{\`E} \gdefchar^^c9{\'E} \gdefchar^^ca{\^E} \gdefchar^^cb{\"E} \gdefchar^^cc{\`I} \gdefchar^^cd{\'I} \gdefchar^^ce{\^I} \gdefchar^^cf{\"I} % \gdefchar^^d0{\DH} \gdefchar^^d1{\~N} \gdefchar^^d2{\`O} \gdefchar^^d3{\'O} \gdefchar^^d4{\^O} \gdefchar^^d5{\~O} \gdefchar^^d6{\"O} \gdefchar^^d7{$\times$} \gdefchar^^d8{\O} \gdefchar^^d9{\`U} \gdefchar^^da{\'U} \gdefchar^^db{\^U} \gdefchar^^dc{\"U} \gdefchar^^dd{\'Y} \gdefchar^^de{\TH} \gdefchar^^df{\ss} % \gdefchar^^e0{\`a} \gdefchar^^e1{\'a} \gdefchar^^e2{\^a} \gdefchar^^e3{\~a} \gdefchar^^e4{\"a} \gdefchar^^e5{\ringaccent a} \gdefchar^^e6{\ae} \gdefchar^^e7{\cedilla c} \gdefchar^^e8{\`e} \gdefchar^^e9{\'e} \gdefchar^^ea{\^e} \gdefchar^^eb{\"e} \gdefchar^^ec{\`{\dotless i}} \gdefchar^^ed{\'{\dotless i}} \gdefchar^^ee{\^{\dotless i}} \gdefchar^^ef{\"{\dotless i}} % \gdefchar^^f0{\dh} \gdefchar^^f1{\~n} \gdefchar^^f2{\`o} \gdefchar^^f3{\'o} \gdefchar^^f4{\^o} \gdefchar^^f5{\~o} \gdefchar^^f6{\"o} \gdefchar^^f7{$\div$} \gdefchar^^f8{\o} \gdefchar^^f9{\`u} \gdefchar^^fa{\'u} \gdefchar^^fb{\^u} \gdefchar^^fc{\"u} \gdefchar^^fd{\'y} \gdefchar^^fe{\th} \gdefchar^^ff{\"y} } % Latin9 (ISO-8859-15) encoding character definitions. \def\latninechardefs{% % Encoding is almost identical to Latin1. \latonechardefs % \gdefchar^^a4{\euro{}} \gdefchar^^a6{\v S} \gdefchar^^a8{\v s} \gdefchar^^b4{\v Z} \gdefchar^^b8{\v z} \gdefchar^^bc{\OE} \gdefchar^^bd{\oe} \gdefchar^^be{\"Y} } % Latin2 (ISO-8859-2) character definitions. \def\lattwochardefs{% \gdefchar^^a0{\tie} \gdefchar^^a1{\ogonek{A}} \gdefchar^^a2{\u{}} \gdefchar^^a3{\L} \gdefchar^^a4{\missingcharmsg{CURRENCY SIGN}} \gdefchar^^a5{\v L} \gdefchar^^a6{\'S} \gdefchar^^a7{\S} \gdefchar^^a8{\"{}} \gdefchar^^a9{\v S} \gdefchar^^aa{\cedilla S} \gdefchar^^ab{\v T} \gdefchar^^ac{\'Z} \gdefchar^^ad{\-} \gdefchar^^ae{\v Z} \gdefchar^^af{\dotaccent Z} % \gdefchar^^b0{\textdegree{}} \gdefchar^^b1{\ogonek{a}} \gdefchar^^b2{\ogonek{ }} \gdefchar^^b3{\l} \gdefchar^^b4{\'{}} \gdefchar^^b5{\v l} \gdefchar^^b6{\'s} \gdefchar^^b7{\v{}} \gdefchar^^b8{\cedilla\ } \gdefchar^^b9{\v s} \gdefchar^^ba{\cedilla s} \gdefchar^^bb{\v t} \gdefchar^^bc{\'z} \gdefchar^^bd{\H{}} \gdefchar^^be{\v z} \gdefchar^^bf{\dotaccent z} % \gdefchar^^c0{\'R} \gdefchar^^c1{\'A} \gdefchar^^c2{\^A} \gdefchar^^c3{\u A} \gdefchar^^c4{\"A} \gdefchar^^c5{\'L} \gdefchar^^c6{\'C} \gdefchar^^c7{\cedilla C} \gdefchar^^c8{\v C} \gdefchar^^c9{\'E} \gdefchar^^ca{\ogonek{E}} \gdefchar^^cb{\"E} \gdefchar^^cc{\v E} \gdefchar^^cd{\'I} \gdefchar^^ce{\^I} \gdefchar^^cf{\v D} % \gdefchar^^d0{\DH} \gdefchar^^d1{\'N} \gdefchar^^d2{\v N} \gdefchar^^d3{\'O} \gdefchar^^d4{\^O} \gdefchar^^d5{\H O} \gdefchar^^d6{\"O} \gdefchar^^d7{$\times$} \gdefchar^^d8{\v R} \gdefchar^^d9{\ringaccent U} \gdefchar^^da{\'U} \gdefchar^^db{\H U} \gdefchar^^dc{\"U} \gdefchar^^dd{\'Y} \gdefchar^^de{\cedilla T} \gdefchar^^df{\ss} % \gdefchar^^e0{\'r} \gdefchar^^e1{\'a} \gdefchar^^e2{\^a} \gdefchar^^e3{\u a} \gdefchar^^e4{\"a} \gdefchar^^e5{\'l} \gdefchar^^e6{\'c} \gdefchar^^e7{\cedilla c} \gdefchar^^e8{\v c} \gdefchar^^e9{\'e} \gdefchar^^ea{\ogonek{e}} \gdefchar^^eb{\"e} \gdefchar^^ec{\v e} \gdefchar^^ed{\'{\dotless{i}}} \gdefchar^^ee{\^{\dotless{i}}} \gdefchar^^ef{\v d} % \gdefchar^^f0{\dh} \gdefchar^^f1{\'n} \gdefchar^^f2{\v n} \gdefchar^^f3{\'o} \gdefchar^^f4{\^o} \gdefchar^^f5{\H o} \gdefchar^^f6{\"o} \gdefchar^^f7{$\div$} \gdefchar^^f8{\v r} \gdefchar^^f9{\ringaccent u} \gdefchar^^fa{\'u} \gdefchar^^fb{\H u} \gdefchar^^fc{\"u} \gdefchar^^fd{\'y} \gdefchar^^fe{\cedilla t} \gdefchar^^ff{\dotaccent{}} } % UTF-8 character definitions. % % This code to support UTF-8 is based on LaTeX's utf8.def, with some % changes for Texinfo conventions. It is included here under the GPL by % permission from Frank Mittelbach and the LaTeX team. % \newcount\countUTFx \newcount\countUTFy \newcount\countUTFz \gdef\UTFviiiTwoOctets#1#2{\expandafter \UTFviiiDefined\csname u8:#1\string #2\endcsname} % \gdef\UTFviiiThreeOctets#1#2#3{\expandafter \UTFviiiDefined\csname u8:#1\string #2\string #3\endcsname} % \gdef\UTFviiiFourOctets#1#2#3#4{\expandafter \UTFviiiDefined\csname u8:#1\string #2\string #3\string #4\endcsname} \gdef\UTFviiiDefined#1{% \ifx #1\relax \message{\linenumber Unicode char \string #1 not defined for Texinfo}% \else \expandafter #1% \fi } % Give non-ASCII bytes the active definitions for processing UTF-8 sequences \begingroup \catcode`\~13 \catcode`\$12 \catcode`\"12 % Loop from \countUTFx to \countUTFy, performing \UTFviiiTmp % substituting ~ and $ with a character token of that value. \def\UTFviiiLoop{% \global\catcode\countUTFx\active \uccode`\~\countUTFx \uccode`\$\countUTFx \uppercase\expandafter{\UTFviiiTmp}% \advance\countUTFx by 1 \ifnum\countUTFx < \countUTFy \expandafter\UTFviiiLoop \fi} % For bytes other than the first in a UTF-8 sequence. Not expected to % be expanded except when writing to auxiliary files. \countUTFx = "80 \countUTFy = "C2 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $\fi}}% \UTFviiiLoop \countUTFx = "C2 \countUTFy = "E0 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $% \else\expandafter\UTFviiiTwoOctets\expandafter$\fi}}% \UTFviiiLoop \countUTFx = "E0 \countUTFy = "F0 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $% \else\expandafter\UTFviiiThreeOctets\expandafter$\fi}}% \UTFviiiLoop \countUTFx = "F0 \countUTFy = "F4 \def\UTFviiiTmp{% \gdef~{% \ifpassthroughchars $% \else\expandafter\UTFviiiFourOctets\expandafter$\fi }}% \UTFviiiLoop \endgroup \def\globallet{\global\let} % save some \expandafter's below % @U{xxxx} to produce U+xxxx, if we support it. \def\U#1{% \expandafter\ifx\csname uni:#1\endcsname \relax \iftxinativeunicodecapable % All Unicode characters can be used if native Unicode handling is % active. However, if the font does not have the glyph, % letters are missing. \begingroup \uccode`\.="#1\relax \uppercase{.} \endgroup \else \errhelp = \EMsimple \errmessage{Unicode character U+#1 not supported, sorry}% \fi \else \csname uni:#1\endcsname \fi } % These macros are used here to construct the name of a control % sequence to be defined. \def\UTFviiiTwoOctetsName#1#2{% \csname u8:#1\string #2\endcsname}% \def\UTFviiiThreeOctetsName#1#2#3{% \csname u8:#1\string #2\string #3\endcsname}% \def\UTFviiiFourOctetsName#1#2#3#4{% \csname u8:#1\string #2\string #3\string #4\endcsname}% % For UTF-8 byte sequences (TeX, e-TeX and pdfTeX), % provide a definition macro to replace a Unicode character; % this gets used by the @U command % \begingroup \catcode`\"=12 \catcode`\<=12 \catcode`\.=12 \catcode`\,=12 \catcode`\;=12 \catcode`\!=12 \catcode`\~=13 \gdef\DeclareUnicodeCharacterUTFviii#1#2{% \countUTFz = "#1\relax \begingroup \parseXMLCharref % Give \u8:... its definition. The sequence of seven \expandafter's % expands after the \gdef three times, e.g. % % 1. \UTFviiTwoOctetsName B1 B2 % 2. \csname u8:B1 \string B2 \endcsname % 3. \u8: B1 B2 (a single control sequence token) % \expandafter\expandafter \expandafter\expandafter \expandafter\expandafter \expandafter\gdef \UTFviiiTmp{#2}% % \expandafter\ifx\csname uni:#1\endcsname \relax \else \message{Internal error, already defined: #1}% \fi % % define an additional control sequence for this code point. \expandafter\globallet\csname uni:#1\endcsname \UTFviiiTmp \endgroup} % % Given the value in \countUTFz as a Unicode code point, set \UTFviiiTmp % to the corresponding UTF-8 sequence. \gdef\parseXMLCharref{% \ifnum\countUTFz < "A0\relax \errhelp = \EMsimple \errmessage{Cannot define Unicode char value < 00A0}% \else\ifnum\countUTFz < "800\relax \parseUTFviiiA,% \parseUTFviiiB C\UTFviiiTwoOctetsName.,% \else\ifnum\countUTFz < "10000\relax \parseUTFviiiA;% \parseUTFviiiA,% \parseUTFviiiB E\UTFviiiThreeOctetsName.{,;}% \else \parseUTFviiiA;% \parseUTFviiiA,% \parseUTFviiiA!% \parseUTFviiiB F\UTFviiiFourOctetsName.{!,;}% \fi\fi\fi } % Extract a byte from the end of the UTF-8 representation of \countUTFx. % It must be a non-initial byte in the sequence. % Change \uccode of #1 for it to be used in \parseUTFviiiB as one % of the bytes. \gdef\parseUTFviiiA#1{% \countUTFx = \countUTFz \divide\countUTFz by 64 \countUTFy = \countUTFz % Save to be the future value of \countUTFz. \multiply\countUTFz by 64 % \countUTFz is now \countUTFx with the last 5 bits cleared. Subtract % in order to get the last five bits. \advance\countUTFx by -\countUTFz % Convert this to the byte in the UTF-8 sequence. \advance\countUTFx by 128 \uccode `#1\countUTFx \countUTFz = \countUTFy} % Used to put a UTF-8 byte sequence into \UTFviiiTmp % #1 is the increment for \countUTFz to yield a the first byte of the UTF-8 % sequence. % #2 is one of the \UTFviii*OctetsName macros. % #3 is always a full stop (.) % #4 is a template for the other bytes in the sequence. The values for these % bytes is substituted in here with \uppercase using the \uccode's. \gdef\parseUTFviiiB#1#2#3#4{% \advance\countUTFz by "#10\relax \uccode `#3\countUTFz \uppercase{\gdef\UTFviiiTmp{#2#3#4}}} \endgroup % For native Unicode handling (XeTeX and LuaTeX), % provide a definition macro that sets a catcode to `other' non-globally % \def\DeclareUnicodeCharacterNativeOther#1#2{% \catcode"#1=\other } % https://en.wikipedia.org/wiki/Plane_(Unicode)#Basic_M % U+0000..U+007F = https://en.wikipedia.org/wiki/Basic_Latin_(Unicode_block) % U+0080..U+00FF = https://en.wikipedia.org/wiki/Latin-1_Supplement_(Unicode_block) % U+0100..U+017F = https://en.wikipedia.org/wiki/Latin_Extended-A % U+0180..U+024F = https://en.wikipedia.org/wiki/Latin_Extended-B % % Many of our renditions are less than wonderful, and all the missing % characters are available somewhere. Loading the necessary fonts % awaits user request. We can't truly support Unicode without % reimplementing everything that's been done in LaTeX for many years, % plus probably using luatex or xetex, and who knows what else. % We won't be doing that here in this simple file. But we can try to at % least make most of the characters not bomb out. % \def\unicodechardefs{% \DeclareUnicodeCharacter{00A0}{\tie}% \DeclareUnicodeCharacter{00A1}{\exclamdown}% \DeclareUnicodeCharacter{00A2}{{\tcfont \char162}}% 0242=cent \DeclareUnicodeCharacter{00A3}{\pounds{}}% \DeclareUnicodeCharacter{00A4}{{\tcfont \char164}}% 0244=currency \DeclareUnicodeCharacter{00A5}{{\tcfont \char165}}% 0245=yen \DeclareUnicodeCharacter{00A6}{{\tcfont \char166}}% 0246=brokenbar \DeclareUnicodeCharacter{00A7}{\S}% \DeclareUnicodeCharacter{00A8}{\"{ }}% \DeclareUnicodeCharacter{00A9}{\copyright{}}% \DeclareUnicodeCharacter{00AA}{\ordf}% \DeclareUnicodeCharacter{00AB}{\guillemetleft{}}% \DeclareUnicodeCharacter{00AC}{\ensuremath\lnot}% \DeclareUnicodeCharacter{00AD}{\-}% \DeclareUnicodeCharacter{00AE}{\registeredsymbol{}}% \DeclareUnicodeCharacter{00AF}{\={ }}% % \DeclareUnicodeCharacter{00B0}{\ringaccent{ }}% \DeclareUnicodeCharacter{00B1}{\ensuremath\pm}% \DeclareUnicodeCharacter{00B2}{$^2$}% \DeclareUnicodeCharacter{00B3}{$^3$}% \DeclareUnicodeCharacter{00B4}{\'{ }}% \DeclareUnicodeCharacter{00B5}{$\mu$}% \DeclareUnicodeCharacter{00B6}{\P}% \DeclareUnicodeCharacter{00B7}{\ensuremath\cdot}% \DeclareUnicodeCharacter{00B8}{\cedilla{ }}% \DeclareUnicodeCharacter{00B9}{$^1$}% \DeclareUnicodeCharacter{00BA}{\ordm}% \DeclareUnicodeCharacter{00BB}{\guillemetright{}}% \DeclareUnicodeCharacter{00BC}{$1\over4$}% \DeclareUnicodeCharacter{00BD}{$1\over2$}% \DeclareUnicodeCharacter{00BE}{$3\over4$}% \DeclareUnicodeCharacter{00BF}{\questiondown}% % \DeclareUnicodeCharacter{00C0}{\`A}% \DeclareUnicodeCharacter{00C1}{\'A}% \DeclareUnicodeCharacter{00C2}{\^A}% \DeclareUnicodeCharacter{00C3}{\~A}% \DeclareUnicodeCharacter{00C4}{\"A}% \DeclareUnicodeCharacter{00C5}{\AA}% \DeclareUnicodeCharacter{00C6}{\AE}% \DeclareUnicodeCharacter{00C7}{\cedilla{C}}% \DeclareUnicodeCharacter{00C8}{\`E}% \DeclareUnicodeCharacter{00C9}{\'E}% \DeclareUnicodeCharacter{00CA}{\^E}% \DeclareUnicodeCharacter{00CB}{\"E}% \DeclareUnicodeCharacter{00CC}{\`I}% \DeclareUnicodeCharacter{00CD}{\'I}% \DeclareUnicodeCharacter{00CE}{\^I}% \DeclareUnicodeCharacter{00CF}{\"I}% % \DeclareUnicodeCharacter{00D0}{\DH}% \DeclareUnicodeCharacter{00D1}{\~N}% \DeclareUnicodeCharacter{00D2}{\`O}% \DeclareUnicodeCharacter{00D3}{\'O}% \DeclareUnicodeCharacter{00D4}{\^O}% \DeclareUnicodeCharacter{00D5}{\~O}% \DeclareUnicodeCharacter{00D6}{\"O}% \DeclareUnicodeCharacter{00D7}{\ensuremath\times}% \DeclareUnicodeCharacter{00D8}{\O}% \DeclareUnicodeCharacter{00D9}{\`U}% \DeclareUnicodeCharacter{00DA}{\'U}% \DeclareUnicodeCharacter{00DB}{\^U}% \DeclareUnicodeCharacter{00DC}{\"U}% \DeclareUnicodeCharacter{00DD}{\'Y}% \DeclareUnicodeCharacter{00DE}{\TH}% \DeclareUnicodeCharacter{00DF}{\ss}% % \DeclareUnicodeCharacter{00E0}{\`a}% \DeclareUnicodeCharacter{00E1}{\'a}% \DeclareUnicodeCharacter{00E2}{\^a}% \DeclareUnicodeCharacter{00E3}{\~a}% \DeclareUnicodeCharacter{00E4}{\"a}% \DeclareUnicodeCharacter{00E5}{\aa}% \DeclareUnicodeCharacter{00E6}{\ae}% \DeclareUnicodeCharacter{00E7}{\cedilla{c}}% \DeclareUnicodeCharacter{00E8}{\`e}% \DeclareUnicodeCharacter{00E9}{\'e}% \DeclareUnicodeCharacter{00EA}{\^e}% \DeclareUnicodeCharacter{00EB}{\"e}% \DeclareUnicodeCharacter{00EC}{\`{\dotless{i}}}% \DeclareUnicodeCharacter{00ED}{\'{\dotless{i}}}% \DeclareUnicodeCharacter{00EE}{\^{\dotless{i}}}% \DeclareUnicodeCharacter{00EF}{\"{\dotless{i}}}% % \DeclareUnicodeCharacter{00F0}{\dh}% \DeclareUnicodeCharacter{00F1}{\~n}% \DeclareUnicodeCharacter{00F2}{\`o}% \DeclareUnicodeCharacter{00F3}{\'o}% \DeclareUnicodeCharacter{00F4}{\^o}% \DeclareUnicodeCharacter{00F5}{\~o}% \DeclareUnicodeCharacter{00F6}{\"o}% \DeclareUnicodeCharacter{00F7}{\ensuremath\div}% \DeclareUnicodeCharacter{00F8}{\o}% \DeclareUnicodeCharacter{00F9}{\`u}% \DeclareUnicodeCharacter{00FA}{\'u}% \DeclareUnicodeCharacter{00FB}{\^u}% \DeclareUnicodeCharacter{00FC}{\"u}% \DeclareUnicodeCharacter{00FD}{\'y}% \DeclareUnicodeCharacter{00FE}{\th}% \DeclareUnicodeCharacter{00FF}{\"y}% % \DeclareUnicodeCharacter{0100}{\=A}% \DeclareUnicodeCharacter{0101}{\=a}% \DeclareUnicodeCharacter{0102}{\u{A}}% \DeclareUnicodeCharacter{0103}{\u{a}}% \DeclareUnicodeCharacter{0104}{\ogonek{A}}% \DeclareUnicodeCharacter{0105}{\ogonek{a}}% \DeclareUnicodeCharacter{0106}{\'C}% \DeclareUnicodeCharacter{0107}{\'c}% \DeclareUnicodeCharacter{0108}{\^C}% \DeclareUnicodeCharacter{0109}{\^c}% \DeclareUnicodeCharacter{010A}{\dotaccent{C}}% \DeclareUnicodeCharacter{010B}{\dotaccent{c}}% \DeclareUnicodeCharacter{010C}{\v{C}}% \DeclareUnicodeCharacter{010D}{\v{c}}% \DeclareUnicodeCharacter{010E}{\v{D}}% \DeclareUnicodeCharacter{010F}{d'}% % \DeclareUnicodeCharacter{0110}{\DH}% \DeclareUnicodeCharacter{0111}{\dh}% \DeclareUnicodeCharacter{0112}{\=E}% \DeclareUnicodeCharacter{0113}{\=e}% \DeclareUnicodeCharacter{0114}{\u{E}}% \DeclareUnicodeCharacter{0115}{\u{e}}% \DeclareUnicodeCharacter{0116}{\dotaccent{E}}% \DeclareUnicodeCharacter{0117}{\dotaccent{e}}% \DeclareUnicodeCharacter{0118}{\ogonek{E}}% \DeclareUnicodeCharacter{0119}{\ogonek{e}}% \DeclareUnicodeCharacter{011A}{\v{E}}% \DeclareUnicodeCharacter{011B}{\v{e}}% \DeclareUnicodeCharacter{011C}{\^G}% \DeclareUnicodeCharacter{011D}{\^g}% \DeclareUnicodeCharacter{011E}{\u{G}}% \DeclareUnicodeCharacter{011F}{\u{g}}% % \DeclareUnicodeCharacter{0120}{\dotaccent{G}}% \DeclareUnicodeCharacter{0121}{\dotaccent{g}}% \DeclareUnicodeCharacter{0122}{\cedilla{G}}% \DeclareUnicodeCharacter{0123}{\cedilla{g}}% \DeclareUnicodeCharacter{0124}{\^H}% \DeclareUnicodeCharacter{0125}{\^h}% \DeclareUnicodeCharacter{0126}{\missingcharmsg{H WITH STROKE}}% \DeclareUnicodeCharacter{0127}{\missingcharmsg{h WITH STROKE}}% \DeclareUnicodeCharacter{0128}{\~I}% \DeclareUnicodeCharacter{0129}{\~{\dotless{i}}}% \DeclareUnicodeCharacter{012A}{\=I}% \DeclareUnicodeCharacter{012B}{\={\dotless{i}}}% \DeclareUnicodeCharacter{012C}{\u{I}}% \DeclareUnicodeCharacter{012D}{\u{\dotless{i}}}% \DeclareUnicodeCharacter{012E}{\ogonek{I}}% \DeclareUnicodeCharacter{012F}{\ogonek{i}}% % \DeclareUnicodeCharacter{0130}{\dotaccent{I}}% \DeclareUnicodeCharacter{0131}{\dotless{i}}% \DeclareUnicodeCharacter{0132}{IJ}% \DeclareUnicodeCharacter{0133}{ij}% \DeclareUnicodeCharacter{0134}{\^J}% \DeclareUnicodeCharacter{0135}{\^{\dotless{j}}}% \DeclareUnicodeCharacter{0136}{\cedilla{K}}% \DeclareUnicodeCharacter{0137}{\cedilla{k}}% \DeclareUnicodeCharacter{0138}{\ensuremath\kappa}% \DeclareUnicodeCharacter{0139}{\'L}% \DeclareUnicodeCharacter{013A}{\'l}% \DeclareUnicodeCharacter{013B}{\cedilla{L}}% \DeclareUnicodeCharacter{013C}{\cedilla{l}}% \DeclareUnicodeCharacter{013D}{L'}% should kern \DeclareUnicodeCharacter{013E}{l'}% should kern \DeclareUnicodeCharacter{013F}{L\U{00B7}}% % \DeclareUnicodeCharacter{0140}{l\U{00B7}}% \DeclareUnicodeCharacter{0141}{\L}% \DeclareUnicodeCharacter{0142}{\l}% \DeclareUnicodeCharacter{0143}{\'N}% \DeclareUnicodeCharacter{0144}{\'n}% \DeclareUnicodeCharacter{0145}{\cedilla{N}}% \DeclareUnicodeCharacter{0146}{\cedilla{n}}% \DeclareUnicodeCharacter{0147}{\v{N}}% \DeclareUnicodeCharacter{0148}{\v{n}}% \DeclareUnicodeCharacter{0149}{'n}% \DeclareUnicodeCharacter{014A}{\missingcharmsg{ENG}}% \DeclareUnicodeCharacter{014B}{\missingcharmsg{eng}}% \DeclareUnicodeCharacter{014C}{\=O}% \DeclareUnicodeCharacter{014D}{\=o}% \DeclareUnicodeCharacter{014E}{\u{O}}% \DeclareUnicodeCharacter{014F}{\u{o}}% % \DeclareUnicodeCharacter{0150}{\H{O}}% \DeclareUnicodeCharacter{0151}{\H{o}}% \DeclareUnicodeCharacter{0152}{\OE}% \DeclareUnicodeCharacter{0153}{\oe}% \DeclareUnicodeCharacter{0154}{\'R}% \DeclareUnicodeCharacter{0155}{\'r}% \DeclareUnicodeCharacter{0156}{\cedilla{R}}% \DeclareUnicodeCharacter{0157}{\cedilla{r}}% \DeclareUnicodeCharacter{0158}{\v{R}}% \DeclareUnicodeCharacter{0159}{\v{r}}% \DeclareUnicodeCharacter{015A}{\'S}% \DeclareUnicodeCharacter{015B}{\'s}% \DeclareUnicodeCharacter{015C}{\^S}% \DeclareUnicodeCharacter{015D}{\^s}% \DeclareUnicodeCharacter{015E}{\cedilla{S}}% \DeclareUnicodeCharacter{015F}{\cedilla{s}}% % \DeclareUnicodeCharacter{0160}{\v{S}}% \DeclareUnicodeCharacter{0161}{\v{s}}% \DeclareUnicodeCharacter{0162}{\cedilla{T}}% \DeclareUnicodeCharacter{0163}{\cedilla{t}}% \DeclareUnicodeCharacter{0164}{\v{T}}% \DeclareUnicodeCharacter{0165}{\v{t}}% \DeclareUnicodeCharacter{0166}{\missingcharmsg{H WITH STROKE}}% \DeclareUnicodeCharacter{0167}{\missingcharmsg{h WITH STROKE}}% \DeclareUnicodeCharacter{0168}{\~U}% \DeclareUnicodeCharacter{0169}{\~u}% \DeclareUnicodeCharacter{016A}{\=U}% \DeclareUnicodeCharacter{016B}{\=u}% \DeclareUnicodeCharacter{016C}{\u{U}}% \DeclareUnicodeCharacter{016D}{\u{u}}% \DeclareUnicodeCharacter{016E}{\ringaccent{U}}% \DeclareUnicodeCharacter{016F}{\ringaccent{u}}% % \DeclareUnicodeCharacter{0170}{\H{U}}% \DeclareUnicodeCharacter{0171}{\H{u}}% \DeclareUnicodeCharacter{0172}{\ogonek{U}}% \DeclareUnicodeCharacter{0173}{\ogonek{u}}% \DeclareUnicodeCharacter{0174}{\^W}% \DeclareUnicodeCharacter{0175}{\^w}% \DeclareUnicodeCharacter{0176}{\^Y}% \DeclareUnicodeCharacter{0177}{\^y}% \DeclareUnicodeCharacter{0178}{\"Y}% \DeclareUnicodeCharacter{0179}{\'Z}% \DeclareUnicodeCharacter{017A}{\'z}% \DeclareUnicodeCharacter{017B}{\dotaccent{Z}}% \DeclareUnicodeCharacter{017C}{\dotaccent{z}}% \DeclareUnicodeCharacter{017D}{\v{Z}}% \DeclareUnicodeCharacter{017E}{\v{z}}% \DeclareUnicodeCharacter{017F}{\missingcharmsg{LONG S}}% % \DeclareUnicodeCharacter{01C4}{D\v{Z}}% \DeclareUnicodeCharacter{01C5}{D\v{z}}% \DeclareUnicodeCharacter{01C6}{d\v{z}}% \DeclareUnicodeCharacter{01C7}{LJ}% \DeclareUnicodeCharacter{01C8}{Lj}% \DeclareUnicodeCharacter{01C9}{lj}% \DeclareUnicodeCharacter{01CA}{NJ}% \DeclareUnicodeCharacter{01CB}{Nj}% \DeclareUnicodeCharacter{01CC}{nj}% \DeclareUnicodeCharacter{01CD}{\v{A}}% \DeclareUnicodeCharacter{01CE}{\v{a}}% \DeclareUnicodeCharacter{01CF}{\v{I}}% % \DeclareUnicodeCharacter{01D0}{\v{\dotless{i}}}% \DeclareUnicodeCharacter{01D1}{\v{O}}% \DeclareUnicodeCharacter{01D2}{\v{o}}% \DeclareUnicodeCharacter{01D3}{\v{U}}% \DeclareUnicodeCharacter{01D4}{\v{u}}% % \DeclareUnicodeCharacter{01E2}{\={\AE}}% \DeclareUnicodeCharacter{01E3}{\={\ae}}% \DeclareUnicodeCharacter{01E6}{\v{G}}% \DeclareUnicodeCharacter{01E7}{\v{g}}% \DeclareUnicodeCharacter{01E8}{\v{K}}% \DeclareUnicodeCharacter{01E9}{\v{k}}% % \DeclareUnicodeCharacter{01F0}{\v{\dotless{j}}}% \DeclareUnicodeCharacter{01F1}{DZ}% \DeclareUnicodeCharacter{01F2}{Dz}% \DeclareUnicodeCharacter{01F3}{dz}% \DeclareUnicodeCharacter{01F4}{\'G}% \DeclareUnicodeCharacter{01F5}{\'g}% \DeclareUnicodeCharacter{01F8}{\`N}% \DeclareUnicodeCharacter{01F9}{\`n}% \DeclareUnicodeCharacter{01FC}{\'{\AE}}% \DeclareUnicodeCharacter{01FD}{\'{\ae}}% \DeclareUnicodeCharacter{01FE}{\'{\O}}% \DeclareUnicodeCharacter{01FF}{\'{\o}}% % \DeclareUnicodeCharacter{021E}{\v{H}}% \DeclareUnicodeCharacter{021F}{\v{h}}% % \DeclareUnicodeCharacter{0226}{\dotaccent{A}}% \DeclareUnicodeCharacter{0227}{\dotaccent{a}}% \DeclareUnicodeCharacter{0228}{\cedilla{E}}% \DeclareUnicodeCharacter{0229}{\cedilla{e}}% \DeclareUnicodeCharacter{022E}{\dotaccent{O}}% \DeclareUnicodeCharacter{022F}{\dotaccent{o}}% % \DeclareUnicodeCharacter{0232}{\=Y}% \DeclareUnicodeCharacter{0233}{\=y}% \DeclareUnicodeCharacter{0237}{\dotless{j}}% % \DeclareUnicodeCharacter{02DB}{\ogonek{ }}% % % Greek letters upper case \DeclareUnicodeCharacter{0391}{{\it A}}% \DeclareUnicodeCharacter{0392}{{\it B}}% \DeclareUnicodeCharacter{0393}{\ensuremath{\mit\Gamma}}% \DeclareUnicodeCharacter{0394}{\ensuremath{\mit\Delta}}% \DeclareUnicodeCharacter{0395}{{\it E}}% \DeclareUnicodeCharacter{0396}{{\it Z}}% \DeclareUnicodeCharacter{0397}{{\it H}}% \DeclareUnicodeCharacter{0398}{\ensuremath{\mit\Theta}}% \DeclareUnicodeCharacter{0399}{{\it I}}% \DeclareUnicodeCharacter{039A}{{\it K}}% \DeclareUnicodeCharacter{039B}{\ensuremath{\mit\Lambda}}% \DeclareUnicodeCharacter{039C}{{\it M}}% \DeclareUnicodeCharacter{039D}{{\it N}}% \DeclareUnicodeCharacter{039E}{\ensuremath{\mit\Xi}}% \DeclareUnicodeCharacter{039F}{{\it O}}% \DeclareUnicodeCharacter{03A0}{\ensuremath{\mit\Pi}}% \DeclareUnicodeCharacter{03A1}{{\it P}}% %\DeclareUnicodeCharacter{03A2}{} % none - corresponds to final sigma \DeclareUnicodeCharacter{03A3}{\ensuremath{\mit\Sigma}}% \DeclareUnicodeCharacter{03A4}{{\it T}}% \DeclareUnicodeCharacter{03A5}{\ensuremath{\mit\Upsilon}}% \DeclareUnicodeCharacter{03A6}{\ensuremath{\mit\Phi}}% \DeclareUnicodeCharacter{03A7}{{\it X}}% \DeclareUnicodeCharacter{03A8}{\ensuremath{\mit\Psi}}% \DeclareUnicodeCharacter{03A9}{\ensuremath{\mit\Omega}}% % % Vowels with accents \DeclareUnicodeCharacter{0390}{\ensuremath{\ddot{\acute\iota}}}% \DeclareUnicodeCharacter{03AC}{\ensuremath{\acute\alpha}}% \DeclareUnicodeCharacter{03AD}{\ensuremath{\acute\epsilon}}% \DeclareUnicodeCharacter{03AE}{\ensuremath{\acute\eta}}% \DeclareUnicodeCharacter{03AF}{\ensuremath{\acute\iota}}% \DeclareUnicodeCharacter{03B0}{\ensuremath{\acute{\ddot\upsilon}}}% % % Standalone accent \DeclareUnicodeCharacter{0384}{\ensuremath{\acute{\ }}}% % % Greek letters lower case \DeclareUnicodeCharacter{03B1}{\ensuremath\alpha}% \DeclareUnicodeCharacter{03B2}{\ensuremath\beta}% \DeclareUnicodeCharacter{03B3}{\ensuremath\gamma}% \DeclareUnicodeCharacter{03B4}{\ensuremath\delta}% \DeclareUnicodeCharacter{03B5}{\ensuremath\epsilon}% \DeclareUnicodeCharacter{03B6}{\ensuremath\zeta}% \DeclareUnicodeCharacter{03B7}{\ensuremath\eta}% \DeclareUnicodeCharacter{03B8}{\ensuremath\theta}% \DeclareUnicodeCharacter{03B9}{\ensuremath\iota}% \DeclareUnicodeCharacter{03BA}{\ensuremath\kappa}% \DeclareUnicodeCharacter{03BB}{\ensuremath\lambda}% \DeclareUnicodeCharacter{03BC}{\ensuremath\mu}% \DeclareUnicodeCharacter{03BD}{\ensuremath\nu}% \DeclareUnicodeCharacter{03BE}{\ensuremath\xi}% \DeclareUnicodeCharacter{03BF}{{\it o}}% omicron \DeclareUnicodeCharacter{03C0}{\ensuremath\pi}% \DeclareUnicodeCharacter{03C1}{\ensuremath\rho}% \DeclareUnicodeCharacter{03C2}{\ensuremath\varsigma}% \DeclareUnicodeCharacter{03C3}{\ensuremath\sigma}% \DeclareUnicodeCharacter{03C4}{\ensuremath\tau}% \DeclareUnicodeCharacter{03C5}{\ensuremath\upsilon}% \DeclareUnicodeCharacter{03C6}{\ensuremath\phi}% \DeclareUnicodeCharacter{03C7}{\ensuremath\chi}% \DeclareUnicodeCharacter{03C8}{\ensuremath\psi}% \DeclareUnicodeCharacter{03C9}{\ensuremath\omega}% % % More Greek vowels with accents \DeclareUnicodeCharacter{03CA}{\ensuremath{\ddot\iota}}% \DeclareUnicodeCharacter{03CB}{\ensuremath{\ddot\upsilon}}% \DeclareUnicodeCharacter{03CC}{\ensuremath{\acute o}}% \DeclareUnicodeCharacter{03CD}{\ensuremath{\acute\upsilon}}% \DeclareUnicodeCharacter{03CE}{\ensuremath{\acute\omega}}% % % Variant Greek letters \DeclareUnicodeCharacter{03D1}{\ensuremath\vartheta}% \DeclareUnicodeCharacter{03D6}{\ensuremath\varpi}% \DeclareUnicodeCharacter{03F1}{\ensuremath\varrho}% % \DeclareUnicodeCharacter{1E02}{\dotaccent{B}}% \DeclareUnicodeCharacter{1E03}{\dotaccent{b}}% \DeclareUnicodeCharacter{1E04}{\udotaccent{B}}% \DeclareUnicodeCharacter{1E05}{\udotaccent{b}}% \DeclareUnicodeCharacter{1E06}{\ubaraccent{B}}% \DeclareUnicodeCharacter{1E07}{\ubaraccent{b}}% \DeclareUnicodeCharacter{1E0A}{\dotaccent{D}}% \DeclareUnicodeCharacter{1E0B}{\dotaccent{d}}% \DeclareUnicodeCharacter{1E0C}{\udotaccent{D}}% \DeclareUnicodeCharacter{1E0D}{\udotaccent{d}}% \DeclareUnicodeCharacter{1E0E}{\ubaraccent{D}}% \DeclareUnicodeCharacter{1E0F}{\ubaraccent{d}}% % \DeclareUnicodeCharacter{1E1E}{\dotaccent{F}}% \DeclareUnicodeCharacter{1E1F}{\dotaccent{f}}% % \DeclareUnicodeCharacter{1E20}{\=G}% \DeclareUnicodeCharacter{1E21}{\=g}% \DeclareUnicodeCharacter{1E22}{\dotaccent{H}}% \DeclareUnicodeCharacter{1E23}{\dotaccent{h}}% \DeclareUnicodeCharacter{1E24}{\udotaccent{H}}% \DeclareUnicodeCharacter{1E25}{\udotaccent{h}}% \DeclareUnicodeCharacter{1E26}{\"H}% \DeclareUnicodeCharacter{1E27}{\"h}% % \DeclareUnicodeCharacter{1E30}{\'K}% \DeclareUnicodeCharacter{1E31}{\'k}% \DeclareUnicodeCharacter{1E32}{\udotaccent{K}}% \DeclareUnicodeCharacter{1E33}{\udotaccent{k}}% \DeclareUnicodeCharacter{1E34}{\ubaraccent{K}}% \DeclareUnicodeCharacter{1E35}{\ubaraccent{k}}% \DeclareUnicodeCharacter{1E36}{\udotaccent{L}}% \DeclareUnicodeCharacter{1E37}{\udotaccent{l}}% \DeclareUnicodeCharacter{1E3A}{\ubaraccent{L}}% \DeclareUnicodeCharacter{1E3B}{\ubaraccent{l}}% \DeclareUnicodeCharacter{1E3E}{\'M}% \DeclareUnicodeCharacter{1E3F}{\'m}% % \DeclareUnicodeCharacter{1E40}{\dotaccent{M}}% \DeclareUnicodeCharacter{1E41}{\dotaccent{m}}% \DeclareUnicodeCharacter{1E42}{\udotaccent{M}}% \DeclareUnicodeCharacter{1E43}{\udotaccent{m}}% \DeclareUnicodeCharacter{1E44}{\dotaccent{N}}% \DeclareUnicodeCharacter{1E45}{\dotaccent{n}}% \DeclareUnicodeCharacter{1E46}{\udotaccent{N}}% \DeclareUnicodeCharacter{1E47}{\udotaccent{n}}% \DeclareUnicodeCharacter{1E48}{\ubaraccent{N}}% \DeclareUnicodeCharacter{1E49}{\ubaraccent{n}}% % \DeclareUnicodeCharacter{1E54}{\'P}% \DeclareUnicodeCharacter{1E55}{\'p}% \DeclareUnicodeCharacter{1E56}{\dotaccent{P}}% \DeclareUnicodeCharacter{1E57}{\dotaccent{p}}% \DeclareUnicodeCharacter{1E58}{\dotaccent{R}}% \DeclareUnicodeCharacter{1E59}{\dotaccent{r}}% \DeclareUnicodeCharacter{1E5A}{\udotaccent{R}}% \DeclareUnicodeCharacter{1E5B}{\udotaccent{r}}% \DeclareUnicodeCharacter{1E5E}{\ubaraccent{R}}% \DeclareUnicodeCharacter{1E5F}{\ubaraccent{r}}% % \DeclareUnicodeCharacter{1E60}{\dotaccent{S}}% \DeclareUnicodeCharacter{1E61}{\dotaccent{s}}% \DeclareUnicodeCharacter{1E62}{\udotaccent{S}}% \DeclareUnicodeCharacter{1E63}{\udotaccent{s}}% \DeclareUnicodeCharacter{1E6A}{\dotaccent{T}}% \DeclareUnicodeCharacter{1E6B}{\dotaccent{t}}% \DeclareUnicodeCharacter{1E6C}{\udotaccent{T}}% \DeclareUnicodeCharacter{1E6D}{\udotaccent{t}}% \DeclareUnicodeCharacter{1E6E}{\ubaraccent{T}}% \DeclareUnicodeCharacter{1E6F}{\ubaraccent{t}}% % \DeclareUnicodeCharacter{1E7C}{\~V}% \DeclareUnicodeCharacter{1E7D}{\~v}% \DeclareUnicodeCharacter{1E7E}{\udotaccent{V}}% \DeclareUnicodeCharacter{1E7F}{\udotaccent{v}}% % \DeclareUnicodeCharacter{1E80}{\`W}% \DeclareUnicodeCharacter{1E81}{\`w}% \DeclareUnicodeCharacter{1E82}{\'W}% \DeclareUnicodeCharacter{1E83}{\'w}% \DeclareUnicodeCharacter{1E84}{\"W}% \DeclareUnicodeCharacter{1E85}{\"w}% \DeclareUnicodeCharacter{1E86}{\dotaccent{W}}% \DeclareUnicodeCharacter{1E87}{\dotaccent{w}}% \DeclareUnicodeCharacter{1E88}{\udotaccent{W}}% \DeclareUnicodeCharacter{1E89}{\udotaccent{w}}% \DeclareUnicodeCharacter{1E8A}{\dotaccent{X}}% \DeclareUnicodeCharacter{1E8B}{\dotaccent{x}}% \DeclareUnicodeCharacter{1E8C}{\"X}% \DeclareUnicodeCharacter{1E8D}{\"x}% \DeclareUnicodeCharacter{1E8E}{\dotaccent{Y}}% \DeclareUnicodeCharacter{1E8F}{\dotaccent{y}}% % \DeclareUnicodeCharacter{1E90}{\^Z}% \DeclareUnicodeCharacter{1E91}{\^z}% \DeclareUnicodeCharacter{1E92}{\udotaccent{Z}}% \DeclareUnicodeCharacter{1E93}{\udotaccent{z}}% \DeclareUnicodeCharacter{1E94}{\ubaraccent{Z}}% \DeclareUnicodeCharacter{1E95}{\ubaraccent{z}}% \DeclareUnicodeCharacter{1E96}{\ubaraccent{h}}% \DeclareUnicodeCharacter{1E97}{\"t}% \DeclareUnicodeCharacter{1E98}{\ringaccent{w}}% \DeclareUnicodeCharacter{1E99}{\ringaccent{y}}% % \DeclareUnicodeCharacter{1EA0}{\udotaccent{A}}% \DeclareUnicodeCharacter{1EA1}{\udotaccent{a}}% % \DeclareUnicodeCharacter{1EB8}{\udotaccent{E}}% \DeclareUnicodeCharacter{1EB9}{\udotaccent{e}}% \DeclareUnicodeCharacter{1EBC}{\~E}% \DeclareUnicodeCharacter{1EBD}{\~e}% % \DeclareUnicodeCharacter{1ECA}{\udotaccent{I}}% \DeclareUnicodeCharacter{1ECB}{\udotaccent{i}}% \DeclareUnicodeCharacter{1ECC}{\udotaccent{O}}% \DeclareUnicodeCharacter{1ECD}{\udotaccent{o}}% % \DeclareUnicodeCharacter{1EE4}{\udotaccent{U}}% \DeclareUnicodeCharacter{1EE5}{\udotaccent{u}}% % \DeclareUnicodeCharacter{1EF2}{\`Y}% \DeclareUnicodeCharacter{1EF3}{\`y}% \DeclareUnicodeCharacter{1EF4}{\udotaccent{Y}}% % \DeclareUnicodeCharacter{1EF8}{\~Y}% \DeclareUnicodeCharacter{1EF9}{\~y}% % % Punctuation \DeclareUnicodeCharacter{2013}{--}% \DeclareUnicodeCharacter{2014}{---}% \DeclareUnicodeCharacter{2018}{\quoteleft{}}% \DeclareUnicodeCharacter{2019}{\quoteright{}}% \DeclareUnicodeCharacter{201A}{\quotesinglbase{}}% \DeclareUnicodeCharacter{201C}{\quotedblleft{}}% \DeclareUnicodeCharacter{201D}{\quotedblright{}}% \DeclareUnicodeCharacter{201E}{\quotedblbase{}}% \DeclareUnicodeCharacter{2020}{\ensuremath\dagger}% \DeclareUnicodeCharacter{2021}{\ensuremath\ddagger}% \DeclareUnicodeCharacter{2022}{\bullet{}}% \DeclareUnicodeCharacter{202F}{\thinspace}% \DeclareUnicodeCharacter{2026}{\dots{}}% \DeclareUnicodeCharacter{2039}{\guilsinglleft{}}% \DeclareUnicodeCharacter{203A}{\guilsinglright{}}% % \DeclareUnicodeCharacter{20AC}{\euro{}}% % \DeclareUnicodeCharacter{2192}{\expansion{}}% \DeclareUnicodeCharacter{21D2}{\result{}}% % % Mathematical symbols \DeclareUnicodeCharacter{2200}{\ensuremath\forall}% \DeclareUnicodeCharacter{2203}{\ensuremath\exists}% \DeclareUnicodeCharacter{2208}{\ensuremath\in}% \DeclareUnicodeCharacter{2212}{\minus{}}% \DeclareUnicodeCharacter{2217}{\ast}% \DeclareUnicodeCharacter{221E}{\ensuremath\infty}% \DeclareUnicodeCharacter{2225}{\ensuremath\parallel}% \DeclareUnicodeCharacter{2227}{\ensuremath\wedge}% \DeclareUnicodeCharacter{2229}{\ensuremath\cap}% \DeclareUnicodeCharacter{2261}{\equiv{}}% \DeclareUnicodeCharacter{2264}{\ensuremath\leq}% \DeclareUnicodeCharacter{2265}{\ensuremath\geq}% \DeclareUnicodeCharacter{2282}{\ensuremath\subset}% \DeclareUnicodeCharacter{2287}{\ensuremath\supseteq}% % \DeclareUnicodeCharacter{2016}{\ensuremath\Vert}% \DeclareUnicodeCharacter{2032}{\ensuremath\prime}% \DeclareUnicodeCharacter{210F}{\ensuremath\hbar}% \DeclareUnicodeCharacter{2111}{\ensuremath\Im}% \DeclareUnicodeCharacter{2113}{\ensuremath\ell}% \DeclareUnicodeCharacter{2118}{\ensuremath\wp}% \DeclareUnicodeCharacter{211C}{\ensuremath\Re}% \DeclareUnicodeCharacter{2135}{\ensuremath\aleph}% \DeclareUnicodeCharacter{2190}{\ensuremath\leftarrow}% \DeclareUnicodeCharacter{2191}{\ensuremath\uparrow}% \DeclareUnicodeCharacter{2193}{\ensuremath\downarrow}% \DeclareUnicodeCharacter{2194}{\ensuremath\leftrightarrow}% \DeclareUnicodeCharacter{2195}{\ensuremath\updownarrow}% \DeclareUnicodeCharacter{2196}{\ensuremath\nwarrow}% \DeclareUnicodeCharacter{2197}{\ensuremath\nearrow}% \DeclareUnicodeCharacter{2198}{\ensuremath\searrow}% \DeclareUnicodeCharacter{2199}{\ensuremath\swarrow}% \DeclareUnicodeCharacter{21A6}{\ensuremath\mapsto}% \DeclareUnicodeCharacter{21A9}{\ensuremath\hookleftarrow}% \DeclareUnicodeCharacter{21AA}{\ensuremath\hookrightarrow}% \DeclareUnicodeCharacter{21BC}{\ensuremath\leftharpoonup}% \DeclareUnicodeCharacter{21BD}{\ensuremath\leftharpoondown}% \DeclareUnicodeCharacter{21C0}{\ensuremath\rightharpoonup}% \DeclareUnicodeCharacter{21C1}{\ensuremath\rightharpoondown}% \DeclareUnicodeCharacter{21CC}{\ensuremath\rightleftharpoons}% \DeclareUnicodeCharacter{21D0}{\ensuremath\Leftarrow}% \DeclareUnicodeCharacter{21D1}{\ensuremath\Uparrow}% \DeclareUnicodeCharacter{21D3}{\ensuremath\Downarrow}% \DeclareUnicodeCharacter{21D4}{\ensuremath\Leftrightarrow}% \DeclareUnicodeCharacter{21D5}{\ensuremath\Updownarrow}% \DeclareUnicodeCharacter{2202}{\ensuremath\partial}% \DeclareUnicodeCharacter{2205}{\ensuremath\emptyset}% \DeclareUnicodeCharacter{2207}{\ensuremath\nabla}% \DeclareUnicodeCharacter{2209}{\ensuremath\notin}% \DeclareUnicodeCharacter{220B}{\ensuremath\owns}% \DeclareUnicodeCharacter{220F}{\ensuremath\prod}% \DeclareUnicodeCharacter{2210}{\ensuremath\coprod}% \DeclareUnicodeCharacter{2211}{\ensuremath\sum}% \DeclareUnicodeCharacter{2213}{\ensuremath\mp}% \DeclareUnicodeCharacter{2218}{\ensuremath\circ}% \DeclareUnicodeCharacter{221A}{\ensuremath\surd}% \DeclareUnicodeCharacter{221D}{\ensuremath\propto}% \DeclareUnicodeCharacter{2220}{\ensuremath\angle}% \DeclareUnicodeCharacter{2223}{\ensuremath\mid}% \DeclareUnicodeCharacter{2228}{\ensuremath\vee}% \DeclareUnicodeCharacter{222A}{\ensuremath\cup}% \DeclareUnicodeCharacter{222B}{\ensuremath\smallint}% \DeclareUnicodeCharacter{222E}{\ensuremath\oint}% \DeclareUnicodeCharacter{223C}{\ensuremath\sim}% \DeclareUnicodeCharacter{2240}{\ensuremath\wr}% \DeclareUnicodeCharacter{2243}{\ensuremath\simeq}% \DeclareUnicodeCharacter{2245}{\ensuremath\cong}% \DeclareUnicodeCharacter{2248}{\ensuremath\approx}% \DeclareUnicodeCharacter{224D}{\ensuremath\asymp}% \DeclareUnicodeCharacter{2250}{\ensuremath\doteq}% \DeclareUnicodeCharacter{2260}{\ensuremath\neq}% \DeclareUnicodeCharacter{226A}{\ensuremath\ll}% \DeclareUnicodeCharacter{226B}{\ensuremath\gg}% \DeclareUnicodeCharacter{227A}{\ensuremath\prec}% \DeclareUnicodeCharacter{227B}{\ensuremath\succ}% \DeclareUnicodeCharacter{2283}{\ensuremath\supset}% \DeclareUnicodeCharacter{2286}{\ensuremath\subseteq}% \DeclareUnicodeCharacter{228E}{\ensuremath\uplus}% \DeclareUnicodeCharacter{2291}{\ensuremath\sqsubseteq}% \DeclareUnicodeCharacter{2292}{\ensuremath\sqsupseteq}% \DeclareUnicodeCharacter{2293}{\ensuremath\sqcap}% \DeclareUnicodeCharacter{2294}{\ensuremath\sqcup}% \DeclareUnicodeCharacter{2295}{\ensuremath\oplus}% \DeclareUnicodeCharacter{2296}{\ensuremath\ominus}% \DeclareUnicodeCharacter{2297}{\ensuremath\otimes}% \DeclareUnicodeCharacter{2298}{\ensuremath\oslash}% \DeclareUnicodeCharacter{2299}{\ensuremath\odot}% \DeclareUnicodeCharacter{22A2}{\ensuremath\vdash}% \DeclareUnicodeCharacter{22A3}{\ensuremath\dashv}% \DeclareUnicodeCharacter{22A4}{\ensuremath\ptextop}% \DeclareUnicodeCharacter{22A5}{\ensuremath\bot}% \DeclareUnicodeCharacter{22A8}{\ensuremath\models}% \DeclareUnicodeCharacter{22C0}{\ensuremath\bigwedge}% \DeclareUnicodeCharacter{22C1}{\ensuremath\bigvee}% \DeclareUnicodeCharacter{22C2}{\ensuremath\bigcap}% \DeclareUnicodeCharacter{22C3}{\ensuremath\bigcup}% \DeclareUnicodeCharacter{22C4}{\ensuremath\diamond}% \DeclareUnicodeCharacter{22C5}{\ensuremath\cdot}% \DeclareUnicodeCharacter{22C6}{\ensuremath\star}% \DeclareUnicodeCharacter{22C8}{\ensuremath\bowtie}% \DeclareUnicodeCharacter{2308}{\ensuremath\lceil}% \DeclareUnicodeCharacter{2309}{\ensuremath\rceil}% \DeclareUnicodeCharacter{230A}{\ensuremath\lfloor}% \DeclareUnicodeCharacter{230B}{\ensuremath\rfloor}% \DeclareUnicodeCharacter{2322}{\ensuremath\frown}% \DeclareUnicodeCharacter{2323}{\ensuremath\smile}% % \DeclareUnicodeCharacter{25B3}{\ensuremath\triangle}% \DeclareUnicodeCharacter{25B7}{\ensuremath\triangleright}% \DeclareUnicodeCharacter{25BD}{\ensuremath\bigtriangledown}% \DeclareUnicodeCharacter{25C1}{\ensuremath\triangleleft}% \DeclareUnicodeCharacter{25C7}{\ensuremath\diamond}% \DeclareUnicodeCharacter{2660}{\ensuremath\spadesuit}% \DeclareUnicodeCharacter{2661}{\ensuremath\heartsuit}% \DeclareUnicodeCharacter{2662}{\ensuremath\diamondsuit}% \DeclareUnicodeCharacter{2663}{\ensuremath\clubsuit}% \DeclareUnicodeCharacter{266D}{\ensuremath\flat}% \DeclareUnicodeCharacter{266E}{\ensuremath\natural}% \DeclareUnicodeCharacter{266F}{\ensuremath\sharp}% \DeclareUnicodeCharacter{26AA}{\ensuremath\bigcirc}% \DeclareUnicodeCharacter{27B9}{\ensuremath\rangle}% \DeclareUnicodeCharacter{27C2}{\ensuremath\perp}% \DeclareUnicodeCharacter{27E8}{\ensuremath\langle}% \DeclareUnicodeCharacter{27F5}{\ensuremath\longleftarrow}% \DeclareUnicodeCharacter{27F6}{\ensuremath\longrightarrow}% \DeclareUnicodeCharacter{27F7}{\ensuremath\longleftrightarrow}% \DeclareUnicodeCharacter{27FC}{\ensuremath\longmapsto}% \DeclareUnicodeCharacter{29F5}{\ensuremath\setminus}% \DeclareUnicodeCharacter{2A00}{\ensuremath\bigodot}% \DeclareUnicodeCharacter{2A01}{\ensuremath\bigoplus}% \DeclareUnicodeCharacter{2A02}{\ensuremath\bigotimes}% \DeclareUnicodeCharacter{2A04}{\ensuremath\biguplus}% \DeclareUnicodeCharacter{2A06}{\ensuremath\bigsqcup}% \DeclareUnicodeCharacter{2A3F}{\ensuremath\amalg}% \DeclareUnicodeCharacter{2AAF}{\ensuremath\preceq}% \DeclareUnicodeCharacter{2AB0}{\ensuremath\succeq}% % \global\mathchardef\checkmark="1370% actually the square root sign \DeclareUnicodeCharacter{2713}{\ensuremath\checkmark}% }% end of \unicodechardefs % UTF-8 byte sequence (pdfTeX) definitions (replacing and @U command) % It makes the setting that replace UTF-8 byte sequence. \def\utfeightchardefs{% \let\DeclareUnicodeCharacter\DeclareUnicodeCharacterUTFviii \unicodechardefs } % Whether the active definitions of non-ASCII characters expand to % non-active tokens with the same character code. This is used to % write characters literally, instead of using active definitions for % printing the correct glyphs. \newif\ifpassthroughchars \passthroughcharsfalse % For native Unicode handling (XeTeX and LuaTeX), % provide a definition macro to replace/pass-through a Unicode character % \def\DeclareUnicodeCharacterNative#1#2{% \catcode"#1=\active \def\dodeclareunicodecharacternative##1##2##3{% \begingroup \uccode`\~="##2\relax \uppercase{\gdef~}{% \ifpassthroughchars ##1% \else ##3% \fi } \endgroup } \begingroup \uccode`\.="#1\relax \uppercase{\def\UTFNativeTmp{.}}% \expandafter\dodeclareunicodecharacternative\UTFNativeTmp{#1}{#2}% \endgroup } % Native Unicode handling (XeTeX and LuaTeX) character replacing definition. % It activates the setting that replaces Unicode characters. \def\nativeunicodechardefs{% \let\DeclareUnicodeCharacter\DeclareUnicodeCharacterNative \unicodechardefs } % For native Unicode handling (XeTeX and LuaTeX), % make the character token expand % to the sequences given in \unicodechardefs for printing. \def\DeclareUnicodeCharacterNativeAtU#1#2{% \def\UTFAtUTmp{#2} \expandafter\globallet\csname uni:#1\endcsname \UTFAtUTmp } % @U command definitions for native Unicode handling (XeTeX and LuaTeX). \def\nativeunicodechardefsatu{% \let\DeclareUnicodeCharacter\DeclareUnicodeCharacterNativeAtU \unicodechardefs } % US-ASCII character definitions. \def\asciichardefs{% nothing need be done \relax } % define all Unicode characters we know about, for the sake of @U. \iftxinativeunicodecapable \nativeunicodechardefsatu \else \utfeightchardefs \fi % Make non-ASCII characters printable again for compatibility with % existing Texinfo documents that may use them, even without declaring a % document encoding. % \setnonasciicharscatcode \other \message{formatting,} \newdimen\defaultparindent \defaultparindent = 15pt \chapheadingskip = 15pt plus 4pt minus 2pt \secheadingskip = 12pt plus 3pt minus 2pt \subsecheadingskip = 9pt plus 2pt minus 2pt % Prevent underfull vbox error messages. \vbadness = 10000 % Don't be very finicky about underfull hboxes, either. \hbadness = 6666 % Following George Bush, get rid of widows and orphans. \widowpenalty=10000 \clubpenalty=10000 % Use TeX 3.0's \emergencystretch to help line breaking, but if we're % using an old version of TeX, don't do anything. We want the amount of % stretch added to depend on the line length, hence the dependence on % \hsize. We call this whenever the paper size is set. % \def\setemergencystretch{% \ifx\emergencystretch\thisisundefined % Allow us to assign to \emergencystretch anyway. \def\emergencystretch{\dimen0}% \else \emergencystretch = .15\hsize \fi } % Parameters in order: 1) textheight; 2) textwidth; % 3) voffset; 4) hoffset; 5) binding offset; 6) topskip; % 7) physical page height; 8) physical page width. % % We also call \setleading{\textleading}, so the caller should define % \textleading. The caller should also set \parskip. % \def\internalpagesizes#1#2#3#4#5#6#7#8{% \voffset = #3\relax \topskip = #6\relax \splittopskip = \topskip % \vsize = #1\relax \advance\vsize by \topskip \outervsize = \vsize \advance\outervsize by 2\topandbottommargin \txipageheight = \vsize % \hsize = #2\relax \outerhsize = \hsize \advance\outerhsize by 0.5in \txipagewidth = \hsize % \normaloffset = #4\relax \bindingoffset = #5\relax % \ifpdf \pdfpageheight #7\relax \pdfpagewidth #8\relax % if we don't reset these, they will remain at "1 true in" of % whatever layout pdftex was dumped with. \pdfhorigin = 1 true in \pdfvorigin = 1 true in \else \ifx\XeTeXrevision\thisisundefined \special{papersize=#8,#7}% \else \pdfpageheight #7\relax \pdfpagewidth #8\relax % XeTeX does not have \pdfhorigin and \pdfvorigin. \fi \fi % \setleading{\textleading} % \parindent = \defaultparindent \setemergencystretch } % @letterpaper (the default). \def\letterpaper{{\globaldefs = 1 \parskip = 3pt plus 2pt minus 1pt \textleading = 13.2pt % % If page is nothing but text, make it come out even. \internalpagesizes{607.2pt}{6in}% that's 46 lines {\voffset}{.25in}% {\bindingoffset}{36pt}% {11in}{8.5in}% }} % Use @smallbook to reset parameters for 7x9.25 trim size. \def\smallbook{{\globaldefs = 1 \parskip = 2pt plus 1pt \textleading = 12pt % \internalpagesizes{7.5in}{5in}% {-.2in}{0in}% {\bindingoffset}{16pt}% {9.25in}{7in}% % \lispnarrowing = 0.3in \tolerance = 700 \contentsrightmargin = 0pt \defbodyindent = .5cm }} % Use @smallerbook to reset parameters for 6x9 trim size. % (Just testing, parameters still in flux.) \def\smallerbook{{\globaldefs = 1 \parskip = 1.5pt plus 1pt \textleading = 12pt % \internalpagesizes{7.4in}{4.8in}% {-.2in}{-.4in}% {0pt}{14pt}% {9in}{6in}% % \lispnarrowing = 0.25in \tolerance = 700 \contentsrightmargin = 0pt \defbodyindent = .4cm }} % Use @afourpaper to print on European A4 paper. \def\afourpaper{{\globaldefs = 1 \parskip = 3pt plus 2pt minus 1pt \textleading = 13.2pt % % Double-side printing via postscript on Laserjet 4050 % prints double-sided nicely when \bindingoffset=10mm and \hoffset=-6mm. % To change the settings for a different printer or situation, adjust % \normaloffset until the front-side and back-side texts align. Then % do the same for \bindingoffset. You can set these for testing in % your texinfo source file like this: % @tex % \global\normaloffset = -6mm % \global\bindingoffset = 10mm % @end tex \internalpagesizes{673.2pt}{160mm}% that's 51 lines {\voffset}{\hoffset}% {\bindingoffset}{44pt}% {297mm}{210mm}% % \tolerance = 700 \contentsrightmargin = 0pt \defbodyindent = 5mm }} % Use @afivepaper to print on European A5 paper. % From romildo@urano.iceb.ufop.br, 2 July 2000. % He also recommends making @example and @lisp be small. \def\afivepaper{{\globaldefs = 1 \parskip = 2pt plus 1pt minus 0.1pt \textleading = 12.5pt % \internalpagesizes{160mm}{120mm}% {\voffset}{\hoffset}% {\bindingoffset}{8pt}% {210mm}{148mm}% % \lispnarrowing = 0.2in \tolerance = 800 \contentsrightmargin = 0pt \defbodyindent = 2mm \tableindent = 12mm }} % A specific text layout, 24x15cm overall, intended for A4 paper. \def\afourlatex{{\globaldefs = 1 \afourpaper \internalpagesizes{237mm}{150mm}% {\voffset}{4.6mm}% {\bindingoffset}{7mm}% {297mm}{210mm}% % % Must explicitly reset to 0 because we call \afourpaper. \globaldefs = 0 }} % Use @afourwide to print on A4 paper in landscape format. \def\afourwide{{\globaldefs = 1 \afourpaper \internalpagesizes{241mm}{165mm}% {\voffset}{-2.95mm}% {\bindingoffset}{7mm}% {297mm}{210mm}% \globaldefs = 0 }} % @pagesizes TEXTHEIGHT[,TEXTWIDTH] % Perhaps we should allow setting the margins, \topskip, \parskip, % and/or leading, also. Or perhaps we should compute them somehow. % \parseargdef\pagesizes{\pagesizesyyy #1,,\finish} \def\pagesizesyyy#1,#2,#3\finish{{% \setbox0 = \hbox{\ignorespaces #2}\ifdim\wd0 > 0pt \hsize=#2\relax \fi \globaldefs = 1 % \parskip = 3pt plus 2pt minus 1pt \setleading{\textleading}% % \dimen0 = #1\relax \advance\dimen0 by \voffset \advance\dimen0 by 1in % reference point for DVI is 1 inch from top of page % \dimen2 = \hsize \advance\dimen2 by \normaloffset \advance\dimen2 by 1in % reference point is 1 inch from left edge of page % \internalpagesizes{#1}{\hsize}% {\voffset}{\normaloffset}% {\bindingoffset}{44pt}% {\dimen0}{\dimen2}% }} % Set default to letter. % \letterpaper % Default value of \hfuzz, for suppressing warnings about overfull hboxes. \hfuzz = 1pt \message{and turning on texinfo input format.} \def^^L{\par} % remove \outer, so ^L can appear in an @comment % DEL is a comment character, in case @c does not suffice. \catcode`\^^? = 14 % Define macros to output various characters with catcode for normal text. \catcode`\"=\other \def\normaldoublequote{"} \catcode`\$=\other \def\normaldollar{$}%$ font-lock fix \catcode`\+=\other \def\normalplus{+} \catcode`\<=\other \def\normalless{<} \catcode`\>=\other \def\normalgreater{>} \catcode`\^=\other \def\normalcaret{^} \catcode`\_=\other \def\normalunderscore{_} \catcode`\|=\other \def\normalverticalbar{|} \catcode`\~=\other \def\normaltilde{~} % This macro is used to make a character print one way in \tt % (where it can probably be output as-is), and another way in other fonts, % where something hairier probably needs to be done. % % #1 is what to print if we are indeed using \tt; #2 is what to print % otherwise. Since all the Computer Modern typewriter fonts have zero % interword stretch (and shrink), and it is reasonable to expect all % typewriter fonts to have this, we can check that font parameter. % \def\ifusingtt#1#2{\ifdim \fontdimen3\font=0pt #1\else #2\fi} % Same as above, but check for italic font. Actually this also catches % non-italic slanted fonts since it is impossible to distinguish them from % italic fonts. But since this is only used by $ and it uses \sl anyway % this is not a problem. \def\ifusingit#1#2{\ifdim \fontdimen1\font>0pt #1\else #2\fi} % Set catcodes for Texinfo file % Active characters for printing the wanted glyph. % Most of these we simply print from the \tt font, but for some, we can % use math or other variants that look better in normal text. % \catcode`\"=\active \def\activedoublequote{{\tt\char34}} \let"=\activedoublequote \catcode`\~=\active \def\activetilde{{\tt\char126}} \let~ = \activetilde \chardef\hatchar=`\^ \catcode`\^=\active \def\activehat{{\tt \hatchar}} \let^ = \activehat \catcode`\_=\active \def_{\ifusingtt\normalunderscore\_} \def\_{\leavevmode \kern.07em \vbox{\hrule width.3em height.1ex}\kern .07em } \let\realunder=_ \catcode`\|=\active \def|{{\tt\char124}} \chardef \less=`\< \catcode`\<=\active \def\activeless{{\tt \less}}\let< = \activeless \chardef \gtr=`\> \catcode`\>=\active \def\activegtr{{\tt \gtr}}\let> = \activegtr \catcode`\+=\active \def+{{\tt \char 43}} \catcode`\$=\active \def${\ifusingit{{\sl\$}}\normaldollar}%$ font-lock fix \catcode`\-=\active \let-=\normaldash % used for headline/footline in the output routine, in case the page % breaks in the middle of an @tex block. \def\texinfochars{% \let< = \activeless \let> = \activegtr \let~ = \activetilde \let^ = \activehat \markupsetuplqdefault \markupsetuprqdefault \let\b = \strong \let\i = \smartitalic % in principle, all other definitions in \tex have to be undone too. } % Used sometimes to turn off (effectively) the active characters even after % parsing them. \def\turnoffactive{% \normalturnoffactive \otherbackslash } \catcode`\@=0 % \backslashcurfont outputs one backslash character in current font, % as in \char`\\. \global\chardef\backslashcurfont=`\\ \global\let\rawbackslashxx=\backslashcurfont % let existing .??s files work % \realbackslash is an actual character `\' with catcode other, and % \doublebackslash is two of them (for the pdf outlines). {\catcode`\\=\other @gdef@realbackslash{\} @gdef@doublebackslash{\\}} % In Texinfo, backslash is an active character; it prints the backslash % in fixed width font. \catcode`\\=\active % @ for escape char from now on. % Print a typewriter backslash. For math mode, we can't simply use % \backslashcurfont: the story here is that in math mode, the \char % of \backslashcurfont ends up printing the roman \ from the math symbol % font (because \char in math mode uses the \mathcode, and plain.tex % sets \mathcode`\\="026E). Hence we use an explicit \mathchar, % which is the decimal equivalent of "715c (class 7, e.g., use \fam; % ignored family value; char position "5C). We can't use " for the % usual hex value because it has already been made active. @def@ttbackslash{{@tt @ifmmode @mathchar29020 @else @backslashcurfont @fi}} @let@backslashchar = @ttbackslash % @backslashchar{} is for user documents. % \rawbackslash defines an active \ to do \backslashcurfont. % \otherbackslash defines an active \ to be a literal `\' character with % catcode other. We switch back and forth between these. @gdef@rawbackslash{@let\=@backslashcurfont} @gdef@otherbackslash{@let\=@realbackslash} % Same as @turnoffactive except outputs \ as {\tt\char`\\} instead of % the literal character `\'. % {@catcode`- = @active @gdef@normalturnoffactive{% @passthroughcharstrue @let-=@normaldash @let"=@normaldoublequote @let$=@normaldollar %$ font-lock fix @let+=@normalplus @let<=@normalless @let>=@normalgreater @let^=@normalcaret @let_=@normalunderscore @let|=@normalverticalbar @let~=@normaltilde @let\=@ttbackslash @markupsetuplqdefault @markupsetuprqdefault @unsepspaces } } % If a .fmt file is being used, characters that might appear in a file % name cannot be active until we have parsed the command line. % So turn them off again, and have @fixbackslash turn them back on. @catcode`+=@other @catcode`@_=@other % \enablebackslashhack - allow file to begin `\input texinfo' % % If a .fmt file is being used, we don't want the `\input texinfo' to show up. % That is what \eatinput is for; after that, the `\' should revert to printing % a backslash. % If the file did not have a `\input texinfo', then it is turned off after % the first line; otherwise the first `\' in the file would cause an error. % This is used on the very last line of this file, texinfo.tex. % We also use @c to call @fixbackslash, in case ends of lines are hidden. { @catcode`@^=7 @catcode`@^^M=13@gdef@enablebackslashhack{% @global@let\ = @eatinput% @catcode`@^^M=13% @def@c{@fixbackslash@c}% % Definition for the newline at the end of this file. @def ^^M{@let^^M@secondlinenl}% % Definition for a newline in the main Texinfo file. @gdef @secondlinenl{@fixbackslash}% % In case the first line has a whole-line command on it @let@originalparsearg@parsearg @def@parsearg{@fixbackslash@originalparsearg} }} {@catcode`@^=7 @catcode`@^^M=13% @gdef@eatinput input texinfo#1^^M{@fixbackslash}} % Emergency active definition of newline, in case an active newline token % appears by mistake. {@catcode`@^=7 @catcode13=13% @gdef@enableemergencynewline{% @gdef^^M{% @par% %<warning: active newline>@par% }}} @gdef@fixbackslash{% @ifx\@eatinput @let\ = @ttbackslash @fi @catcode13=5 % regular end of line @enableemergencynewline @let@c=@texinfoc @let@parsearg@originalparsearg % Also turn back on active characters that might appear in the input % file name, in case not using a pre-dumped format. @catcode`+=@active @catcode`@_=@active % % If texinfo.cnf is present on the system, read it. % Useful for site-wide @afourpaper, etc. This macro, @fixbackslash, gets % called at the beginning of every Texinfo file. Not opening texinfo.cnf % directly in this file, texinfo.tex, makes it possible to make a format % file for Texinfo. % @openin 1 texinfo.cnf @ifeof 1 @else @input texinfo.cnf @fi @closein 1 } % Say @foo, not \foo, in error messages. @escapechar = `@@ % These (along with & and #) are made active for url-breaking, so need % active definitions as the normal characters. @def@normaldot{.} @def@normalquest{?} @def@normalslash{/} % These look ok in all fonts, so just make them not special. % @hashchar{} gets its own user-level command, because of #line. @catcode`@& = @other @def@normalamp{&} @catcode`@# = @other @def@normalhash{#} @catcode`@% = @other @def@normalpercent{%} @let @hashchar = @normalhash @c Finally, make ` and ' active, so that txicodequoteundirected and @c txicodequotebacktick work right in, e.g., @w{@code{`foo'}}. If we @c don't make ` and ' active, @code will not get them as active chars. @c Do this last of all since we use ` in the previous @catcode assignments. @catcode`@'=@active @catcode`@`=@active @markupsetuplqdefault @markupsetuprqdefault @c Local variables: @c eval: (add-hook 'write-file-hooks 'time-stamp) @c page-delimiter: "^\\\\message\\|emacs-page" @c time-stamp-start: "def\\\\texinfoversion{" @c time-stamp-format: "%:y-%02m-%02d.%02H" @c time-stamp-end: "}" @c End: @c vim:sw=2: @enablebackslashhack ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bootstrapped/build-aux/mdate-sh��������������������������������������������������������0000755�0001750�0001750�00000013732�13163446446�016212� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������#!/bin/sh # Get modification time of a file or directory and pretty-print it. scriptversion=2017-09-22.02; # UTC # Copyright (C) 1995-2017 Free Software Foundation, Inc. # written by Ulrich Drepper <drepper@gnu.ai.mit.edu>, June 1995 # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2, or (at your option) # any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see <https://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to <bug-automake@gnu.org> or send patches to # <automake-patches@gnu.org>. if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: # Pre-4.2 versions of Zsh do word splitting on ${1+"$@"}, which # is contrary to our usage. Disable this feature. alias -g '${1+"$@"}'='"$@"' setopt NO_GLOB_SUBST fi case $1 in '') echo "$0: No file. Try '$0 --help' for more information." 1>&2 exit 1; ;; -h | --h*) cat <<\EOF Usage: mdate-sh [--help] [--version] FILE Pretty-print the modification day of FILE, in the format: 1 January 1970 Report bugs to <bug-automake@gnu.org>. EOF exit $? ;; -v | --v*) echo "mdate-sh $scriptversion" exit $? ;; esac error () { echo "$0: $1" >&2 exit 1 } # Prevent date giving response in another language. LANG=C export LANG LC_ALL=C export LC_ALL LC_TIME=C export LC_TIME # Use UTC to get reproducible result. TZ=UTC0 export TZ # GNU ls changes its time format in response to the TIME_STYLE # variable. Since we cannot assume 'unset' works, revert this # variable to its documented default. if test "${TIME_STYLE+set}" = set; then TIME_STYLE=posix-long-iso export TIME_STYLE fi save_arg1=$1 # Find out how to get the extended ls output of a file or directory. if ls -L /dev/null 1>/dev/null 2>&1; then ls_command='ls -L -l -d' else ls_command='ls -l -d' fi # Avoid user/group names that might have spaces, when possible. if ls -n /dev/null 1>/dev/null 2>&1; then ls_command="$ls_command -n" fi # A 'ls -l' line looks as follows on OS/2. # drwxrwx--- 0 Aug 11 2001 foo # This differs from Unix, which adds ownership information. # drwxrwx--- 2 root root 4096 Aug 11 2001 foo # # To find the date, we split the line on spaces and iterate on words # until we find a month. This cannot work with files whose owner is a # user named "Jan", or "Feb", etc. However, it's unlikely that '/' # will be owned by a user whose name is a month. So we first look at # the extended ls output of the root directory to decide how many # words should be skipped to get the date. # On HPUX /bin/sh, "set" interprets "-rw-r--r--" as options, so the "x" below. set x`$ls_command /` # Find which argument is the month. month= command= until test $month do test $# -gt 0 || error "failed parsing '$ls_command /' output" shift # Add another shift to the command. command="$command shift;" case $1 in Jan) month=January; nummonth=1;; Feb) month=February; nummonth=2;; Mar) month=March; nummonth=3;; Apr) month=April; nummonth=4;; May) month=May; nummonth=5;; Jun) month=June; nummonth=6;; Jul) month=July; nummonth=7;; Aug) month=August; nummonth=8;; Sep) month=September; nummonth=9;; Oct) month=October; nummonth=10;; Nov) month=November; nummonth=11;; Dec) month=December; nummonth=12;; esac done test -n "$month" || error "failed parsing '$ls_command /' output" # Get the extended ls output of the file or directory. set dummy x`eval "$ls_command \"\\\$save_arg1\""` # Remove all preceding arguments eval $command # Because of the dummy argument above, month is in $2. # # On a POSIX system, we should have # # $# = 5 # $1 = file size # $2 = month # $3 = day # $4 = year or time # $5 = filename # # On Darwin 7.7.0 and 7.6.0, we have # # $# = 4 # $1 = day # $2 = month # $3 = year or time # $4 = filename # Get the month. case $2 in Jan) month=January; nummonth=1;; Feb) month=February; nummonth=2;; Mar) month=March; nummonth=3;; Apr) month=April; nummonth=4;; May) month=May; nummonth=5;; Jun) month=June; nummonth=6;; Jul) month=July; nummonth=7;; Aug) month=August; nummonth=8;; Sep) month=September; nummonth=9;; Oct) month=October; nummonth=10;; Nov) month=November; nummonth=11;; Dec) month=December; nummonth=12;; esac case $3 in ???*) day=$1;; *) day=$3; shift;; esac # Here we have to deal with the problem that the ls output gives either # the time of day or the year. case $3 in *:*) set `date`; eval year=\$$# case $2 in Jan) nummonthtod=1;; Feb) nummonthtod=2;; Mar) nummonthtod=3;; Apr) nummonthtod=4;; May) nummonthtod=5;; Jun) nummonthtod=6;; Jul) nummonthtod=7;; Aug) nummonthtod=8;; Sep) nummonthtod=9;; Oct) nummonthtod=10;; Nov) nummonthtod=11;; Dec) nummonthtod=12;; esac # For the first six month of the year the time notation can also # be used for files modified in the last year. if (expr $nummonth \> $nummonthtod) > /dev/null; then year=`expr $year - 1` fi;; *) year=$3;; esac # The result. echo $day $month $year # Local Variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "scriptversion=" # time-stamp-format: "%:y-%02m-%02d.%02H" # time-stamp-time-zone: "UTC0" # time-stamp-end: "; # UTC" # End: ��������������������������������������gnuastro-0.5/bootstrapped/build-aux/depcomp���������������������������������������������������������0000755�0001750�0001750�00000056020�13163446446�016134� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������#! /bin/sh # depcomp - compile a program generating dependencies as side-effects scriptversion=2017-09-16.17; # UTC # Copyright (C) 1999-2017 Free Software Foundation, Inc. # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2, or (at your option) # any later version. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # You should have received a copy of the GNU General Public License # along with this program. If not, see <https://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # Originally written by Alexandre Oliva <oliva@dcc.unicamp.br>. case $1 in '') echo "$0: No command. Try '$0 --help' for more information." 1>&2 exit 1; ;; -h | --h*) cat <<\EOF Usage: depcomp [--help] [--version] PROGRAM [ARGS] Run PROGRAMS ARGS to compile a file, generating dependencies as side-effects. Environment variables: depmode Dependency tracking mode. source Source file read by 'PROGRAMS ARGS'. object Object file output by 'PROGRAMS ARGS'. DEPDIR directory where to store dependencies. depfile Dependency file to output. tmpdepfile Temporary file to use when outputting dependencies. libtool Whether libtool is used (yes/no). Report bugs to <bug-automake@gnu.org>. EOF exit $? ;; -v | --v*) echo "depcomp $scriptversion" exit $? ;; esac # Get the directory component of the given path, and save it in the # global variables '$dir'. Note that this directory component will # be either empty or ending with a '/' character. This is deliberate. set_dir_from () { case $1 in */*) dir=`echo "$1" | sed -e 's|/[^/]*$|/|'`;; *) dir=;; esac } # Get the suffix-stripped basename of the given path, and save it the # global variable '$base'. set_base_from () { base=`echo "$1" | sed -e 's|^.*/||' -e 's/\.[^.]*$//'` } # If no dependency file was actually created by the compiler invocation, # we still have to create a dummy depfile, to avoid errors with the # Makefile "include basename.Plo" scheme. make_dummy_depfile () { echo "#dummy" > "$depfile" } # Factor out some common post-processing of the generated depfile. # Requires the auxiliary global variable '$tmpdepfile' to be set. aix_post_process_depfile () { # If the compiler actually managed to produce a dependency file, # post-process it. if test -f "$tmpdepfile"; then # Each line is of the form 'foo.o: dependency.h'. # Do two passes, one to just change these to # $object: dependency.h # and one to simply output # dependency.h: # which is needed to avoid the deleted-header problem. { sed -e "s,^.*\.[$lower]*:,$object:," < "$tmpdepfile" sed -e "s,^.*\.[$lower]*:[$tab ]*,," -e 's,$,:,' < "$tmpdepfile" } > "$depfile" rm -f "$tmpdepfile" else make_dummy_depfile fi } # A tabulation character. tab=' ' # A newline character. nl=' ' # Character ranges might be problematic outside the C locale. # These definitions help. upper=ABCDEFGHIJKLMNOPQRSTUVWXYZ lower=abcdefghijklmnopqrstuvwxyz digits=0123456789 alpha=${upper}${lower} if test -z "$depmode" || test -z "$source" || test -z "$object"; then echo "depcomp: Variables source, object and depmode must be set" 1>&2 exit 1 fi # Dependencies for sub/bar.o or sub/bar.obj go into sub/.deps/bar.Po. depfile=${depfile-`echo "$object" | sed 's|[^\\/]*$|'${DEPDIR-.deps}'/&|;s|\.\([^.]*\)$|.P\1|;s|Pobj$|Po|'`} tmpdepfile=${tmpdepfile-`echo "$depfile" | sed 's/\.\([^.]*\)$/.T\1/'`} rm -f "$tmpdepfile" # Avoid interferences from the environment. gccflag= dashmflag= # Some modes work just like other modes, but use different flags. We # parameterize here, but still list the modes in the big case below, # to make depend.m4 easier to write. Note that we *cannot* use a case # here, because this file can only contain one case statement. if test "$depmode" = hp; then # HP compiler uses -M and no extra arg. gccflag=-M depmode=gcc fi if test "$depmode" = dashXmstdout; then # This is just like dashmstdout with a different argument. dashmflag=-xM depmode=dashmstdout fi cygpath_u="cygpath -u -f -" if test "$depmode" = msvcmsys; then # This is just like msvisualcpp but w/o cygpath translation. # Just convert the backslash-escaped backslashes to single forward # slashes to satisfy depend.m4 cygpath_u='sed s,\\\\,/,g' depmode=msvisualcpp fi if test "$depmode" = msvc7msys; then # This is just like msvc7 but w/o cygpath translation. # Just convert the backslash-escaped backslashes to single forward # slashes to satisfy depend.m4 cygpath_u='sed s,\\\\,/,g' depmode=msvc7 fi if test "$depmode" = xlc; then # IBM C/C++ Compilers xlc/xlC can output gcc-like dependency information. gccflag=-qmakedep=gcc,-MF depmode=gcc fi case "$depmode" in gcc3) ## gcc 3 implements dependency tracking that does exactly what ## we want. Yay! Note: for some reason libtool 1.4 doesn't like ## it if -MD -MP comes after the -MF stuff. Hmm. ## Unfortunately, FreeBSD c89 acceptance of flags depends upon ## the command line argument order; so add the flags where they ## appear in depend2.am. Note that the slowdown incurred here ## affects only configure: in makefiles, %FASTDEP% shortcuts this. for arg do case $arg in -c) set fnord "$@" -MT "$object" -MD -MP -MF "$tmpdepfile" "$arg" ;; *) set fnord "$@" "$arg" ;; esac shift # fnord shift # $arg done "$@" stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi mv "$tmpdepfile" "$depfile" ;; gcc) ## Note that this doesn't just cater to obsosete pre-3.x GCC compilers. ## but also to in-use compilers like IMB xlc/xlC and the HP C compiler. ## (see the conditional assignment to $gccflag above). ## There are various ways to get dependency output from gcc. Here's ## why we pick this rather obscure method: ## - Don't want to use -MD because we'd like the dependencies to end ## up in a subdir. Having to rename by hand is ugly. ## (We might end up doing this anyway to support other compilers.) ## - The DEPENDENCIES_OUTPUT environment variable makes gcc act like ## -MM, not -M (despite what the docs say). Also, it might not be ## supported by the other compilers which use the 'gcc' depmode. ## - Using -M directly means running the compiler twice (even worse ## than renaming). if test -z "$gccflag"; then gccflag=-MD, fi "$@" -Wp,"$gccflag$tmpdepfile" stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi rm -f "$depfile" echo "$object : \\" > "$depfile" # The second -e expression handles DOS-style file names with drive # letters. sed -e 's/^[^:]*: / /' \ -e 's/^['$alpha']:\/[^:]*: / /' < "$tmpdepfile" >> "$depfile" ## This next piece of magic avoids the "deleted header file" problem. ## The problem is that when a header file which appears in a .P file ## is deleted, the dependency causes make to die (because there is ## typically no way to rebuild the header). We avoid this by adding ## dummy dependencies for each header file. Too bad gcc doesn't do ## this for us directly. ## Some versions of gcc put a space before the ':'. On the theory ## that the space means something, we add a space to the output as ## well. hp depmode also adds that space, but also prefixes the VPATH ## to the object. Take care to not repeat it in the output. ## Some versions of the HPUX 10.20 sed can't process this invocation ## correctly. Breaking it into two sed invocations is a workaround. tr ' ' "$nl" < "$tmpdepfile" \ | sed -e 's/^\\$//' -e '/^$/d' -e "s|.*$object$||" -e '/:$/d' \ | sed -e 's/$/ :/' >> "$depfile" rm -f "$tmpdepfile" ;; hp) # This case exists only to let depend.m4 do its work. It works by # looking at the text of this script. This case will never be run, # since it is checked for above. exit 1 ;; sgi) if test "$libtool" = yes; then "$@" "-Wp,-MDupdate,$tmpdepfile" else "$@" -MDupdate "$tmpdepfile" fi stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi rm -f "$depfile" if test -f "$tmpdepfile"; then # yes, the sourcefile depend on other files echo "$object : \\" > "$depfile" # Clip off the initial element (the dependent). Don't try to be # clever and replace this with sed code, as IRIX sed won't handle # lines with more than a fixed number of characters (4096 in # IRIX 6.2 sed, 8192 in IRIX 6.5). We also remove comment lines; # the IRIX cc adds comments like '#:fec' to the end of the # dependency line. tr ' ' "$nl" < "$tmpdepfile" \ | sed -e 's/^.*\.o://' -e 's/#.*$//' -e '/^$/ d' \ | tr "$nl" ' ' >> "$depfile" echo >> "$depfile" # The second pass generates a dummy entry for each header file. tr ' ' "$nl" < "$tmpdepfile" \ | sed -e 's/^.*\.o://' -e 's/#.*$//' -e '/^$/ d' -e 's/$/:/' \ >> "$depfile" else make_dummy_depfile fi rm -f "$tmpdepfile" ;; xlc) # This case exists only to let depend.m4 do its work. It works by # looking at the text of this script. This case will never be run, # since it is checked for above. exit 1 ;; aix) # The C for AIX Compiler uses -M and outputs the dependencies # in a .u file. In older versions, this file always lives in the # current directory. Also, the AIX compiler puts '$object:' at the # start of each line; $object doesn't have directory information. # Version 6 uses the directory in both cases. set_dir_from "$object" set_base_from "$object" if test "$libtool" = yes; then tmpdepfile1=$dir$base.u tmpdepfile2=$base.u tmpdepfile3=$dir.libs/$base.u "$@" -Wc,-M else tmpdepfile1=$dir$base.u tmpdepfile2=$dir$base.u tmpdepfile3=$dir$base.u "$@" -M fi stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile1" "$tmpdepfile2" "$tmpdepfile3" exit $stat fi for tmpdepfile in "$tmpdepfile1" "$tmpdepfile2" "$tmpdepfile3" do test -f "$tmpdepfile" && break done aix_post_process_depfile ;; tcc) # tcc (Tiny C Compiler) understand '-MD -MF file' since version 0.9.26 # FIXME: That version still under development at the moment of writing. # Make that this statement remains true also for stable, released # versions. # It will wrap lines (doesn't matter whether long or short) with a # trailing '\', as in: # # foo.o : \ # foo.c \ # foo.h \ # # It will put a trailing '\' even on the last line, and will use leading # spaces rather than leading tabs (at least since its commit 0394caf7 # "Emit spaces for -MD"). "$@" -MD -MF "$tmpdepfile" stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi rm -f "$depfile" # Each non-empty line is of the form 'foo.o : \' or ' dep.h \'. # We have to change lines of the first kind to '$object: \'. sed -e "s|.*:|$object :|" < "$tmpdepfile" > "$depfile" # And for each line of the second kind, we have to emit a 'dep.h:' # dummy dependency, to avoid the deleted-header problem. sed -n -e 's|^ *\(.*\) *\\$|\1:|p' < "$tmpdepfile" >> "$depfile" rm -f "$tmpdepfile" ;; ## The order of this option in the case statement is important, since the ## shell code in configure will try each of these formats in the order ## listed in this file. A plain '-MD' option would be understood by many ## compilers, so we must ensure this comes after the gcc and icc options. pgcc) # Portland's C compiler understands '-MD'. # Will always output deps to 'file.d' where file is the root name of the # source file under compilation, even if file resides in a subdirectory. # The object file name does not affect the name of the '.d' file. # pgcc 10.2 will output # foo.o: sub/foo.c sub/foo.h # and will wrap long lines using '\' : # foo.o: sub/foo.c ... \ # sub/foo.h ... \ # ... set_dir_from "$object" # Use the source, not the object, to determine the base name, since # that's sadly what pgcc will do too. set_base_from "$source" tmpdepfile=$base.d # For projects that build the same source file twice into different object # files, the pgcc approach of using the *source* file root name can cause # problems in parallel builds. Use a locking strategy to avoid stomping on # the same $tmpdepfile. lockdir=$base.d-lock trap " echo '$0: caught signal, cleaning up...' >&2 rmdir '$lockdir' exit 1 " 1 2 13 15 numtries=100 i=$numtries while test $i -gt 0; do # mkdir is a portable test-and-set. if mkdir "$lockdir" 2>/dev/null; then # This process acquired the lock. "$@" -MD stat=$? # Release the lock. rmdir "$lockdir" break else # If the lock is being held by a different process, wait # until the winning process is done or we timeout. while test -d "$lockdir" && test $i -gt 0; do sleep 1 i=`expr $i - 1` done fi i=`expr $i - 1` done trap - 1 2 13 15 if test $i -le 0; then echo "$0: failed to acquire lock after $numtries attempts" >&2 echo "$0: check lockdir '$lockdir'" >&2 exit 1 fi if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi rm -f "$depfile" # Each line is of the form `foo.o: dependent.h', # or `foo.o: dep1.h dep2.h \', or ` dep3.h dep4.h \'. # Do two passes, one to just change these to # `$object: dependent.h' and one to simply `dependent.h:'. sed "s,^[^:]*:,$object :," < "$tmpdepfile" > "$depfile" # Some versions of the HPUX 10.20 sed can't process this invocation # correctly. Breaking it into two sed invocations is a workaround. sed 's,^[^:]*: \(.*\)$,\1,;s/^\\$//;/^$/d;/:$/d' < "$tmpdepfile" \ | sed -e 's/$/ :/' >> "$depfile" rm -f "$tmpdepfile" ;; hp2) # The "hp" stanza above does not work with aCC (C++) and HP's ia64 # compilers, which have integrated preprocessors. The correct option # to use with these is +Maked; it writes dependencies to a file named # 'foo.d', which lands next to the object file, wherever that # happens to be. # Much of this is similar to the tru64 case; see comments there. set_dir_from "$object" set_base_from "$object" if test "$libtool" = yes; then tmpdepfile1=$dir$base.d tmpdepfile2=$dir.libs/$base.d "$@" -Wc,+Maked else tmpdepfile1=$dir$base.d tmpdepfile2=$dir$base.d "$@" +Maked fi stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile1" "$tmpdepfile2" exit $stat fi for tmpdepfile in "$tmpdepfile1" "$tmpdepfile2" do test -f "$tmpdepfile" && break done if test -f "$tmpdepfile"; then sed -e "s,^.*\.[$lower]*:,$object:," "$tmpdepfile" > "$depfile" # Add 'dependent.h:' lines. sed -ne '2,${ s/^ *// s/ \\*$// s/$/:/ p }' "$tmpdepfile" >> "$depfile" else make_dummy_depfile fi rm -f "$tmpdepfile" "$tmpdepfile2" ;; tru64) # The Tru64 compiler uses -MD to generate dependencies as a side # effect. 'cc -MD -o foo.o ...' puts the dependencies into 'foo.o.d'. # At least on Alpha/Redhat 6.1, Compaq CCC V6.2-504 seems to put # dependencies in 'foo.d' instead, so we check for that too. # Subdirectories are respected. set_dir_from "$object" set_base_from "$object" if test "$libtool" = yes; then # Libtool generates 2 separate objects for the 2 libraries. These # two compilations output dependencies in $dir.libs/$base.o.d and # in $dir$base.o.d. We have to check for both files, because # one of the two compilations can be disabled. We should prefer # $dir$base.o.d over $dir.libs/$base.o.d because the latter is # automatically cleaned when .libs/ is deleted, while ignoring # the former would cause a distcleancheck panic. tmpdepfile1=$dir$base.o.d # libtool 1.5 tmpdepfile2=$dir.libs/$base.o.d # Likewise. tmpdepfile3=$dir.libs/$base.d # Compaq CCC V6.2-504 "$@" -Wc,-MD else tmpdepfile1=$dir$base.d tmpdepfile2=$dir$base.d tmpdepfile3=$dir$base.d "$@" -MD fi stat=$? if test $stat -ne 0; then rm -f "$tmpdepfile1" "$tmpdepfile2" "$tmpdepfile3" exit $stat fi for tmpdepfile in "$tmpdepfile1" "$tmpdepfile2" "$tmpdepfile3" do test -f "$tmpdepfile" && break done # Same post-processing that is required for AIX mode. aix_post_process_depfile ;; msvc7) if test "$libtool" = yes; then showIncludes=-Wc,-showIncludes else showIncludes=-showIncludes fi "$@" $showIncludes > "$tmpdepfile" stat=$? grep -v '^Note: including file: ' "$tmpdepfile" if test $stat -ne 0; then rm -f "$tmpdepfile" exit $stat fi rm -f "$depfile" echo "$object : \\" > "$depfile" # The first sed program below extracts the file names and escapes # backslashes for cygpath. The second sed program outputs the file # name when reading, but also accumulates all include files in the # hold buffer in order to output them again at the end. This only # works with sed implementations that can handle large buffers. sed < "$tmpdepfile" -n ' /^Note: including file: *\(.*\)/ { s//\1/ s/\\/\\\\/g p }' | $cygpath_u | sort -u | sed -n ' s/ /\\ /g s/\(.*\)/'"$tab"'\1 \\/p s/.\(.*\) \\/\1:/ H $ { s/.*/'"$tab"'/ G p }' >> "$depfile" echo >> "$depfile" # make sure the fragment doesn't end with a backslash rm -f "$tmpdepfile" ;; msvc7msys) # This case exists only to let depend.m4 do its work. It works by # looking at the text of this script. This case will never be run, # since it is checked for above. exit 1 ;; #nosideeffect) # This comment above is used by automake to tell side-effect # dependency tracking mechanisms from slower ones. dashmstdout) # Important note: in order to support this mode, a compiler *must* # always write the preprocessed file to stdout, regardless of -o. "$@" || exit $? # Remove the call to Libtool. if test "$libtool" = yes; then while test "X$1" != 'X--mode=compile'; do shift done shift fi # Remove '-o $object'. IFS=" " for arg do case $arg in -o) shift ;; $object) shift ;; *) set fnord "$@" "$arg" shift # fnord shift # $arg ;; esac done test -z "$dashmflag" && dashmflag=-M # Require at least two characters before searching for ':' # in the target name. This is to cope with DOS-style filenames: # a dependency such as 'c:/foo/bar' could be seen as target 'c' otherwise. "$@" $dashmflag | sed "s|^[$tab ]*[^:$tab ][^:][^:]*:[$tab ]*|$object: |" > "$tmpdepfile" rm -f "$depfile" cat < "$tmpdepfile" > "$depfile" # Some versions of the HPUX 10.20 sed can't process this sed invocation # correctly. Breaking it into two sed invocations is a workaround. tr ' ' "$nl" < "$tmpdepfile" \ | sed -e 's/^\\$//' -e '/^$/d' -e '/:$/d' \ | sed -e 's/$/ :/' >> "$depfile" rm -f "$tmpdepfile" ;; dashXmstdout) # This case only exists to satisfy depend.m4. It is never actually # run, as this mode is specially recognized in the preamble. exit 1 ;; makedepend) "$@" || exit $? # Remove any Libtool call if test "$libtool" = yes; then while test "X$1" != 'X--mode=compile'; do shift done shift fi # X makedepend shift cleared=no eat=no for arg do case $cleared in no) set ""; shift cleared=yes ;; esac if test $eat = yes; then eat=no continue fi case "$arg" in -D*|-I*) set fnord "$@" "$arg"; shift ;; # Strip any option that makedepend may not understand. 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"$@" || exit $? # Remove the call to Libtool. if test "$libtool" = yes; then while test "X$1" != 'X--mode=compile'; do shift done shift fi # Remove '-o $object'. IFS=" " for arg do case $arg in -o) shift ;; $object) shift ;; *) set fnord "$@" "$arg" shift # fnord shift # $arg ;; esac done "$@" -E \ | sed -n -e '/^# [0-9][0-9]* "\([^"]*\)".*/ s:: \1 \\:p' \ -e '/^#line [0-9][0-9]* "\([^"]*\)".*/ s:: \1 \\:p' \ | sed '$ s: \\$::' > "$tmpdepfile" rm -f "$depfile" echo "$object : \\" > "$depfile" cat < "$tmpdepfile" >> "$depfile" sed < "$tmpdepfile" '/^$/d;s/^ //;s/ \\$//;s/$/ :/' >> "$depfile" rm -f "$tmpdepfile" ;; msvisualcpp) # Important note: in order to support this mode, a compiler *must* # always write the preprocessed file to stdout. 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PROGRAM=libtool PACKAGE=libtool VERSION=2.4.6.40-6ca5-dirty package_revision=2.4.6.40 ## ------ ## ## Usage. ## ## ------ ## # Run './libtool --help' for help with using this script from the # command line. ## ------------------------------- ## ## User overridable command paths. ## ## ------------------------------- ## # After configure completes, it has a better idea of some of the # shell tools we need than the defaults used by the functions shared # with bootstrap, so set those here where they can still be over- # ridden by the user, but otherwise take precedence. : ${AUTOCONF="autoconf"} : ${AUTOMAKE="automake"} ## -------------------------- ## ## Source external libraries. ## ## -------------------------- ## # Much of our low-level functionality needs to be sourced from external # libraries, which are installed to $pkgauxdir. # Set a version string for this script. scriptversion=2017-04-19.12; # UTC # General shell script boiler plate, and helper functions. # Written by Gary V. 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See the URLs above, or the file `LICENSE` # included in the Bootstrap distribution for the full license texts. # Please report bugs or propose patches to: # <https://github.com/gnulib-modules/bootstrap/issues> ## ------ ## ## Usage. ## ## ------ ## # Evaluate this file near the top of your script to gain access to # the functions and variables defined here: # # . `echo "$0" | ${SED-sed} 's|[^/]*$||'`/build-aux/funclib.sh # # If you need to override any of the default environment variable # settings, do that before evaluating this file. ## -------------------- ## ## Shell normalisation. ## ## -------------------- ## # Some shells need a little help to be as Bourne compatible as possible. # Before doing anything else, make sure all that help has been provided! DUALCASE=1; export DUALCASE # for MKS sh if test -n "${ZSH_VERSION+set}" && (emulate sh) >/dev/null 2>&1; then : emulate sh NULLCMD=: # Pre-4.2 versions of Zsh do word splitting on ${1+"$@"}, which # is contrary to our usage. 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(eval unset $1) >/dev/null 2>&1 && eval unset $1 || : ; } } # Make sure CDPATH doesn't cause `cd` commands to output the target dir. func_unset CDPATH # Make sure ${,E,F}GREP behave sanely. func_unset GREP_OPTIONS ## ------------------------- ## ## Locate command utilities. ## ## ------------------------- ## # func_executable_p FILE # ---------------------- # Check that FILE is an executable regular file. func_executable_p () { test -f "$1" && test -x "$1" } # func_path_progs PROGS_LIST CHECK_FUNC [PATH] # -------------------------------------------- # Search for either a program that responds to --version with output # containing "GNU", or else returned by CHECK_FUNC otherwise, by # trying all the directories in PATH with each of the elements of # PROGS_LIST. # # CHECK_FUNC should accept the path to a candidate program, and # set $func_check_prog_result if it truncates its output less than # $_G_path_prog_max characters. func_path_progs () { _G_progs_list=$1 _G_check_func=$2 _G_PATH=${3-"$PATH"} _G_path_prog_max=0 _G_path_prog_found=false _G_save_IFS=$IFS; 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do _G_sed_script=$_G_sed_script$nl$_G_sed_script done echo "$_G_sed_script" 2>/dev/null | sed 99q >conftest.sed _G_sed_script= func_check_prog_sed () { _G_path_prog=$1 _G_count=0 printf 0123456789 >conftest.in while : do cat conftest.in conftest.in >conftest.tmp mv conftest.tmp conftest.in cp conftest.in conftest.nl echo '' >> conftest.nl "$_G_path_prog" -f conftest.sed <conftest.nl >conftest.out 2>/dev/null || break diff conftest.out conftest.nl >/dev/null 2>&1 || break _G_count=`expr $_G_count + 1` if test "$_G_count" -gt "$_G_path_prog_max"; then # Best one so far, save it but keep looking for a better one func_check_prog_result=$_G_path_prog _G_path_prog_max=$_G_count fi # 10*(2^10) chars as input seems more than enough test 10 -lt "$_G_count" && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out } func_path_progs "sed gsed" func_check_prog_sed "$PATH:/usr/xpg4/bin" rm -f conftest.sed SED=$func_path_progs_result } # Unless the user overrides by setting GREP, search the path for either GNU # grep, or the grep that truncates its output the least. test -z "$GREP" && { func_check_prog_grep () { _G_path_prog=$1 _G_count=0 _G_path_prog_max=0 printf 0123456789 >conftest.in while : do cat conftest.in conftest.in >conftest.tmp mv conftest.tmp conftest.in cp conftest.in conftest.nl echo 'GREP' >> conftest.nl "$_G_path_prog" -e 'GREP$' -e '-(cannot match)-' <conftest.nl >conftest.out 2>/dev/null || break diff conftest.out conftest.nl >/dev/null 2>&1 || break _G_count=`expr $_G_count + 1` if test "$_G_count" -gt "$_G_path_prog_max"; then # Best one so far, save it but keep looking for a better one func_check_prog_result=$_G_path_prog _G_path_prog_max=$_G_count fi # 10*(2^10) chars as input seems more than enough test 10 -lt "$_G_count" && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out } func_path_progs "grep ggrep" func_check_prog_grep "$PATH:/usr/xpg4/bin" GREP=$func_path_progs_result } ## ------------------------------- ## ## User overridable command paths. ## ## ------------------------------- ## # All uppercase variable names are used for environment variables. These # variables can be overridden by the user before calling a script that # uses them if a suitable command of that name is not already available # in the command search PATH. : ${CP="cp -f"} : ${ECHO="printf %s\n"} : ${EGREP="$GREP -E"} : ${FGREP="$GREP -F"} : ${LN_S="ln -s"} : ${MAKE="make"} : ${MKDIR="mkdir"} : ${MV="mv -f"} : ${RM="rm -f"} : ${SHELL="${CONFIG_SHELL-/bin/sh}"} ## -------------------- ## ## Useful sed snippets. ## ## -------------------- ## sed_dirname='s|/[^/]*$||' sed_basename='s|^.*/||' # Sed substitution that helps us do robust quoting. It backslashifies # metacharacters that are still active within double-quoted strings. sed_quote_subst='s|\([`"$\\]\)|\\\1|g' # Same as above, but do not quote variable references. sed_double_quote_subst='s/\(["`\\]\)/\\\1/g' # Sed substitution that turns a string into a regex matching for the # string literally. sed_make_literal_regex='s|[].[^$\\*\/]|\\&|g' # Sed substitution that converts a w32 file name or path # that contains forward slashes, into one that contains # (escaped) backslashes. A very naive implementation. sed_naive_backslashify='s|\\\\*|\\|g;s|/|\\|g;s|\\|\\\\|g' # Re-'\' parameter expansions in output of sed_double_quote_subst that # were '\'-ed in input to the same. If an odd number of '\' preceded a # '$' in input to sed_double_quote_subst, that '$' was protected from # expansion. Since each input '\' is now two '\'s, look for any number # of runs of four '\'s followed by two '\'s and then a '$'. '\' that '$'. _G_bs='\\' _G_bs2='\\\\' _G_bs4='\\\\\\\\' _G_dollar='\$' sed_double_backslash="\ s/$_G_bs4/&\\ /g s/^$_G_bs2$_G_dollar/$_G_bs&/ s/\\([^$_G_bs]\\)$_G_bs2$_G_dollar/\\1$_G_bs2$_G_bs$_G_dollar/g s/\n//g" ## ----------------- ## ## Global variables. ## ## ----------------- ## # Except for the global variables explicitly listed below, the following # functions in the '^func_' namespace, and the '^require_' namespace # variables initialised in the 'Resource management' section, sourcing # this file will not pollute your global namespace with anything # else. There's no portable way to scope variables in Bourne shell # though, so actually running these functions will sometimes place # results into a variable named after the function, and often use # temporary variables in the '^_G_' namespace. If you are careful to # avoid using those namespaces casually in your sourcing script, things # should continue to work as you expect. And, of course, you can freely # overwrite any of the functions or variables defined here before # calling anything to customize them. EXIT_SUCCESS=0 EXIT_FAILURE=1 EXIT_MISMATCH=63 # $? = 63 is used to indicate version mismatch to missing. EXIT_SKIP=77 # $? = 77 is used to indicate a skipped test to automake. # Allow overriding, eg assuming that you follow the convention of # putting '$debug_cmd' at the start of all your functions, you can get # bash to show function call trace with: # # debug_cmd='eval echo "${FUNCNAME[0]} $*" >&2' bash your-script-name debug_cmd=${debug_cmd-":"} exit_cmd=: # By convention, finish your script with: # # exit $exit_status # # so that you can set exit_status to non-zero if you want to indicate # something went wrong during execution without actually bailing out at # the point of failure. exit_status=$EXIT_SUCCESS # Work around backward compatibility issue on IRIX 6.5. On IRIX 6.4+, sh # is ksh but when the shell is invoked as "sh" and the current value of # the _XPG environment variable is not equal to 1 (one), the special # positional parameter $0, within a function call, is the name of the # function. progpath=$0 # The name of this program. progname=`$ECHO "$progpath" |$SED "$sed_basename"` # Make sure we have an absolute progpath for reexecution: case $progpath in [\\/]*|[A-Za-z]:\\*) ;; *[\\/]*) progdir=`$ECHO "$progpath" |$SED "$sed_dirname"` progdir=`cd "$progdir" && pwd` progpath=$progdir/$progname ;; *) _G_IFS=$IFS IFS=${PATH_SEPARATOR-:} for progdir in $PATH; do IFS=$_G_IFS test -x "$progdir/$progname" && break done IFS=$_G_IFS test -n "$progdir" || progdir=`pwd` progpath=$progdir/$progname ;; esac ## ----------------- ## ## Standard options. ## ## ----------------- ## # The following options affect the operation of the functions defined # below, and should be set appropriately depending on run-time para- # meters passed on the command line. opt_dry_run=false opt_quiet=false opt_verbose=false # Categories 'all' and 'none' are always available. Append any others # you will pass as the first argument to func_warning from your own # code. warning_categories= # By default, display warnings according to 'opt_warning_types'. Set # 'warning_func' to ':' to elide all warnings, or func_fatal_error to # treat the next displayed warning as a fatal error. warning_func=func_warn_and_continue # Set to 'all' to display all warnings, 'none' to suppress all # warnings, or a space delimited list of some subset of # 'warning_categories' to display only the listed warnings. opt_warning_types=all ## -------------------- ## ## Resource management. ## ## -------------------- ## # This section contains definitions for functions that each ensure a # particular resource (a file, or a non-empty configuration variable for # example) is available, and if appropriate to extract default values # from pertinent package files. Call them using their associated # 'require_*' variable to ensure that they are executed, at most, once. # # It's entirely deliberate that calling these functions can set # variables that don't obey the namespace limitations obeyed by the rest # of this file, in order that that they be as useful as possible to # callers. # require_term_colors # ------------------- # Allow display of bold text on terminals that support it. require_term_colors=func_require_term_colors func_require_term_colors () { $debug_cmd test -t 1 && { # COLORTERM and USE_ANSI_COLORS environment variables take # precedence, because most terminfo databases neglect to describe # whether color sequences are supported. test -n "${COLORTERM+set}" && : ${USE_ANSI_COLORS="1"} if test 1 = "$USE_ANSI_COLORS"; then # Standard ANSI escape sequences tc_reset='' tc_bold=''; tc_standout='' tc_red=''; tc_green='' tc_blue=''; tc_cyan='' else # Otherwise trust the terminfo database after all. test -n "`tput sgr0 2>/dev/null`" && { tc_reset=`tput sgr0` test -n "`tput bold 2>/dev/null`" && tc_bold=`tput bold` tc_standout=$tc_bold test -n "`tput smso 2>/dev/null`" && tc_standout=`tput smso` test -n "`tput setaf 1 2>/dev/null`" && tc_red=`tput setaf 1` test -n "`tput setaf 2 2>/dev/null`" && tc_green=`tput setaf 2` test -n "`tput setaf 4 2>/dev/null`" && tc_blue=`tput setaf 4` test -n "`tput setaf 5 2>/dev/null`" && tc_cyan=`tput setaf 5` } fi } require_term_colors=: } ## ----------------- ## ## Function library. ## ## ----------------- ## # This section contains a variety of useful functions to call in your # scripts. Take note of the portable wrappers for features provided by # some modern shells, which will fall back to slower equivalents on # less featureful shells. # func_append VAR VALUE # --------------------- # Append VALUE onto the existing contents of VAR. # We should try to minimise forks, especially on Windows where they are # unreasonably slow, so skip the feature probes when bash or zsh are # being used: if test set = "${BASH_VERSION+set}${ZSH_VERSION+set}"; then : ${_G_HAVE_ARITH_OP="yes"} : ${_G_HAVE_XSI_OPS="yes"} # The += operator was introduced in bash 3.1 case $BASH_VERSION in [12].* | 3.0 | 3.0*) ;; *) : ${_G_HAVE_PLUSEQ_OP="yes"} ;; esac fi # _G_HAVE_PLUSEQ_OP # Can be empty, in which case the shell is probed, "yes" if += is # useable or anything else if it does not work. test -z "$_G_HAVE_PLUSEQ_OP" \ && (eval 'x=a; x+=" b"; test "a b" = "$x"') 2>/dev/null \ && _G_HAVE_PLUSEQ_OP=yes if test yes = "$_G_HAVE_PLUSEQ_OP" then # This is an XSI compatible shell, allowing a faster implementation... eval 'func_append () { $debug_cmd eval "$1+=\$2" }' else # ...otherwise fall back to using expr, which is often a shell builtin. func_append () { $debug_cmd eval "$1=\$$1\$2" } fi # func_append_quoted VAR VALUE # ---------------------------- # Quote VALUE and append to the end of shell variable VAR, separated # by a space. if test yes = "$_G_HAVE_PLUSEQ_OP"; then eval 'func_append_quoted () { $debug_cmd func_quote_arg pretty "$2" eval "$1+=\\ \$func_quote_arg_result" }' else func_append_quoted () { $debug_cmd func_quote_arg pretty "$2" eval "$1=\$$1\\ \$func_quote_arg_result" } fi # func_append_uniq VAR VALUE # -------------------------- # Append unique VALUE onto the existing contents of VAR, assuming # entries are delimited by the first character of VALUE. For example: # # func_append_uniq options " --another-option option-argument" # # will only append to $options if " --another-option option-argument " # is not already present somewhere in $options already (note spaces at # each end implied by leading space in second argument). func_append_uniq () { $debug_cmd eval _G_current_value='`$ECHO $'$1'`' _G_delim=`expr "$2" : '\(.\)'` case $_G_delim$_G_current_value$_G_delim in *"$2$_G_delim"*) ;; *) func_append "$@" ;; esac } # func_arith TERM... # ------------------ # Set func_arith_result to the result of evaluating TERMs. test -z "$_G_HAVE_ARITH_OP" \ && (eval 'test 2 = $(( 1 + 1 ))') 2>/dev/null \ && _G_HAVE_ARITH_OP=yes if test yes = "$_G_HAVE_ARITH_OP"; then eval 'func_arith () { $debug_cmd func_arith_result=$(( $* )) }' else func_arith () { $debug_cmd func_arith_result=`expr "$@"` } fi # func_basename FILE # ------------------ # Set func_basename_result to FILE with everything up to and including # the last / stripped. if test yes = "$_G_HAVE_XSI_OPS"; then # If this shell supports suffix pattern removal, then use it to avoid # forking. Hide the definitions single quotes in case the shell chokes # on unsupported syntax... _b='func_basename_result=${1##*/}' _d='case $1 in */*) func_dirname_result=${1%/*}$2 ;; * ) func_dirname_result=$3 ;; esac' else # ...otherwise fall back to using sed. _b='func_basename_result=`$ECHO "$1" |$SED "$sed_basename"`' _d='func_dirname_result=`$ECHO "$1" |$SED "$sed_dirname"` if test "X$func_dirname_result" = "X$1"; then func_dirname_result=$3 else func_append func_dirname_result "$2" fi' fi eval 'func_basename () { $debug_cmd '"$_b"' }' # func_dirname FILE APPEND NONDIR_REPLACEMENT # ------------------------------------------- # Compute the dirname of FILE. If nonempty, add APPEND to the result, # otherwise set result to NONDIR_REPLACEMENT. eval 'func_dirname () { $debug_cmd '"$_d"' }' # func_dirname_and_basename FILE APPEND NONDIR_REPLACEMENT # -------------------------------------------------------- # Perform func_basename and func_dirname in a single function # call: # dirname: Compute the dirname of FILE. If nonempty, # add APPEND to the result, otherwise set result # to NONDIR_REPLACEMENT. # value returned in "$func_dirname_result" # basename: Compute filename of FILE. # value retuned in "$func_basename_result" # For efficiency, we do not delegate to the functions above but instead # duplicate the functionality here. eval 'func_dirname_and_basename () { $debug_cmd '"$_b"' '"$_d"' }' # func_echo ARG... # ---------------- # Echo program name prefixed message. func_echo () { $debug_cmd _G_message=$* func_echo_IFS=$IFS IFS=$nl for _G_line in $_G_message; do IFS=$func_echo_IFS $ECHO "$progname: $_G_line" done IFS=$func_echo_IFS } # func_echo_all ARG... # -------------------- # Invoke $ECHO with all args, space-separated. func_echo_all () { $ECHO "$*" } # func_echo_infix_1 INFIX ARG... # ------------------------------ # Echo program name, followed by INFIX on the first line, with any # additional lines not showing INFIX. func_echo_infix_1 () { $debug_cmd $require_term_colors _G_infix=$1; shift _G_indent=$_G_infix _G_prefix="$progname: $_G_infix: " _G_message=$* # Strip color escape sequences before counting printable length for _G_tc in "$tc_reset" "$tc_bold" "$tc_standout" "$tc_red" "$tc_green" "$tc_blue" "$tc_cyan" do test -n "$_G_tc" && { _G_esc_tc=`$ECHO "$_G_tc" | $SED "$sed_make_literal_regex"` _G_indent=`$ECHO "$_G_indent" | $SED "s|$_G_esc_tc||g"` } done _G_indent="$progname: "`echo "$_G_indent" | $SED 's|.| |g'`" " ## exclude from sc_prohibit_nested_quotes func_echo_infix_1_IFS=$IFS IFS=$nl for _G_line in $_G_message; do IFS=$func_echo_infix_1_IFS $ECHO "$_G_prefix$tc_bold$_G_line$tc_reset" >&2 _G_prefix=$_G_indent done IFS=$func_echo_infix_1_IFS } # func_error ARG... # ----------------- # Echo program name prefixed message to standard error. func_error () { $debug_cmd $require_term_colors func_echo_infix_1 " $tc_standout${tc_red}error$tc_reset" "$*" >&2 } # func_fatal_error ARG... # ----------------------- # Echo program name prefixed message to standard error, and exit. func_fatal_error () { $debug_cmd func_error "$*" exit $EXIT_FAILURE } # func_grep EXPRESSION FILENAME # ----------------------------- # Check whether EXPRESSION matches any line of FILENAME, without output. func_grep () { $debug_cmd $GREP "$1" "$2" >/dev/null 2>&1 } # func_len STRING # --------------- # Set func_len_result to the length of STRING. STRING may not # start with a hyphen. test -z "$_G_HAVE_XSI_OPS" \ && (eval 'x=a/b/c; test 5aa/bb/cc = "${#x}${x%%/*}${x%/*}${x#*/}${x##*/}"') 2>/dev/null \ && _G_HAVE_XSI_OPS=yes if test yes = "$_G_HAVE_XSI_OPS"; then eval 'func_len () { $debug_cmd func_len_result=${#1} }' else func_len () { $debug_cmd func_len_result=`expr "$1" : ".*" 2>/dev/null || echo $max_cmd_len` } fi # func_mkdir_p DIRECTORY-PATH # --------------------------- # Make sure the entire path to DIRECTORY-PATH is available. func_mkdir_p () { $debug_cmd _G_directory_path=$1 _G_dir_list= if test -n "$_G_directory_path" && test : != "$opt_dry_run"; then # Protect directory names starting with '-' case $_G_directory_path in -*) _G_directory_path=./$_G_directory_path ;; esac # While some portion of DIR does not yet exist... while test ! -d "$_G_directory_path"; do # ...make a list in topmost first order. Use a colon delimited # list incase some portion of path contains whitespace. _G_dir_list=$_G_directory_path:$_G_dir_list # If the last portion added has no slash in it, the list is done case $_G_directory_path in */*) ;; *) break ;; esac # ...otherwise throw away the child directory and loop _G_directory_path=`$ECHO "$_G_directory_path" | $SED -e "$sed_dirname"` done _G_dir_list=`$ECHO "$_G_dir_list" | $SED 's|:*$||'` func_mkdir_p_IFS=$IFS; IFS=: for _G_dir in $_G_dir_list; do IFS=$func_mkdir_p_IFS # mkdir can fail with a 'File exist' error if two processes # try to create one of the directories concurrently. Don't # stop in that case! $MKDIR "$_G_dir" 2>/dev/null || : done IFS=$func_mkdir_p_IFS # Bail out if we (or some other process) failed to create a directory. test -d "$_G_directory_path" || \ func_fatal_error "Failed to create '$1'" fi } # func_mktempdir [BASENAME] # ------------------------- # Make a temporary directory that won't clash with other running # libtool processes, and avoids race conditions if possible. If # given, BASENAME is the basename for that directory. func_mktempdir () { $debug_cmd _G_template=${TMPDIR-/tmp}/${1-$progname} if test : = "$opt_dry_run"; then # Return a directory name, but don't create it in dry-run mode _G_tmpdir=$_G_template-$$ else # If mktemp works, use that first and foremost _G_tmpdir=`mktemp -d "$_G_template-XXXXXXXX" 2>/dev/null` if test ! -d "$_G_tmpdir"; then # Failing that, at least try and use $RANDOM to avoid a race _G_tmpdir=$_G_template-${RANDOM-0}$$ func_mktempdir_umask=`umask` umask 0077 $MKDIR "$_G_tmpdir" umask $func_mktempdir_umask fi # If we're not in dry-run mode, bomb out on failure test -d "$_G_tmpdir" || \ func_fatal_error "cannot create temporary directory '$_G_tmpdir'" fi $ECHO "$_G_tmpdir" } # func_normal_abspath PATH # ------------------------ # Remove doubled-up and trailing slashes, "." path components, # and cancel out any ".." path components in PATH after making # it an absolute path. func_normal_abspath () { $debug_cmd # These SED scripts presuppose an absolute path with a trailing slash. _G_pathcar='s|^/\([^/]*\).*$|\1|' _G_pathcdr='s|^/[^/]*||' _G_removedotparts=':dotsl s|/\./|/|g t dotsl s|/\.$|/|' _G_collapseslashes='s|/\{1,\}|/|g' _G_finalslash='s|/*$|/|' # Start from root dir and reassemble the path. func_normal_abspath_result= func_normal_abspath_tpath=$1 func_normal_abspath_altnamespace= case $func_normal_abspath_tpath in "") # Empty path, that just means $cwd. func_stripname '' '/' "`pwd`" func_normal_abspath_result=$func_stripname_result return ;; # The next three entries are used to spot a run of precisely # two leading slashes without using negated character classes; # we take advantage of case's first-match behaviour. ///*) # Unusual form of absolute path, do nothing. ;; //*) # Not necessarily an ordinary path; POSIX reserves leading '//' # and for example Cygwin uses it to access remote file shares # over CIFS/SMB, so we conserve a leading double slash if found. func_normal_abspath_altnamespace=/ ;; /*) # Absolute path, do nothing. ;; *) # Relative path, prepend $cwd. func_normal_abspath_tpath=`pwd`/$func_normal_abspath_tpath ;; esac # Cancel out all the simple stuff to save iterations. We also want # the path to end with a slash for ease of parsing, so make sure # there is one (and only one) here. func_normal_abspath_tpath=`$ECHO "$func_normal_abspath_tpath" | $SED \ -e "$_G_removedotparts" -e "$_G_collapseslashes" -e "$_G_finalslash"` while :; do # Processed it all yet? if test / = "$func_normal_abspath_tpath"; then # If we ascended to the root using ".." the result may be empty now. if test -z "$func_normal_abspath_result"; then func_normal_abspath_result=/ fi break fi func_normal_abspath_tcomponent=`$ECHO "$func_normal_abspath_tpath" | $SED \ -e "$_G_pathcar"` func_normal_abspath_tpath=`$ECHO "$func_normal_abspath_tpath" | $SED \ -e "$_G_pathcdr"` # Figure out what to do with it case $func_normal_abspath_tcomponent in "") # Trailing empty path component, ignore it. ;; ..) # Parent dir; strip last assembled component from result. func_dirname "$func_normal_abspath_result" func_normal_abspath_result=$func_dirname_result ;; *) # Actual path component, append it. func_append func_normal_abspath_result "/$func_normal_abspath_tcomponent" ;; esac done # Restore leading double-slash if one was found on entry. func_normal_abspath_result=$func_normal_abspath_altnamespace$func_normal_abspath_result } # func_notquiet ARG... # -------------------- # Echo program name prefixed message only when not in quiet mode. func_notquiet () { $debug_cmd $opt_quiet || func_echo ${1+"$@"} # A bug in bash halts the script if the last line of a function # fails when set -e is in force, so we need another command to # work around that: : } # func_relative_path SRCDIR DSTDIR # -------------------------------- # Set func_relative_path_result to the relative path from SRCDIR to DSTDIR. func_relative_path () { $debug_cmd func_relative_path_result= func_normal_abspath "$1" func_relative_path_tlibdir=$func_normal_abspath_result func_normal_abspath "$2" func_relative_path_tbindir=$func_normal_abspath_result # Ascend the tree starting from libdir while :; do # check if we have found a prefix of bindir case $func_relative_path_tbindir in $func_relative_path_tlibdir) # found an exact match func_relative_path_tcancelled= break ;; $func_relative_path_tlibdir*) # found a matching prefix func_stripname "$func_relative_path_tlibdir" '' "$func_relative_path_tbindir" func_relative_path_tcancelled=$func_stripname_result if test -z "$func_relative_path_result"; then func_relative_path_result=. fi break ;; *) func_dirname $func_relative_path_tlibdir func_relative_path_tlibdir=$func_dirname_result if test -z "$func_relative_path_tlibdir"; then # Have to descend all the way to the root! func_relative_path_result=../$func_relative_path_result func_relative_path_tcancelled=$func_relative_path_tbindir break fi func_relative_path_result=../$func_relative_path_result ;; esac done # Now calculate path; take care to avoid doubling-up slashes. func_stripname '' '/' "$func_relative_path_result" func_relative_path_result=$func_stripname_result func_stripname '/' '/' "$func_relative_path_tcancelled" if test -n "$func_stripname_result"; then func_append func_relative_path_result "/$func_stripname_result" fi # Normalisation. If bindir is libdir, return '.' else relative path. if test -n "$func_relative_path_result"; then func_stripname './' '' "$func_relative_path_result" func_relative_path_result=$func_stripname_result fi test -n "$func_relative_path_result" || func_relative_path_result=. : } # func_quote_portable EVAL ARG # ---------------------------- # Internal function to portably implement func_quote_arg. Note that we still # keep attention to performance here so we as much as possible try to avoid # calling sed binary (so far O(N) complexity as long as func_append is O(1)). func_quote_portable () { $debug_cmd func_quote_portable_result=$2 # one-time-loop (easy break) while true do if $1; then func_quote_portable_result=`$ECHO "$2" | $SED \ -e "$sed_double_quote_subst" -e "$sed_double_backslash"` break fi # Quote for eval. case $func_quote_portable_result in *[\\\`\"\$]*) case $func_quote_portable_result in *[\[\*\?]*) func_quote_portable_result=`$ECHO "$func_quote_portable_result" \ | $SED "$sed_quote_subst"` break ;; esac func_quote_portable_old_IFS=$IFS for _G_char in '\' '`' '"' '$' do # STATE($1) PREV($2) SEPARATOR($3) set start "" "" func_quote_portable_result=dummy"$_G_char$func_quote_portable_result$_G_char"dummy IFS=$_G_char for _G_part in $func_quote_portable_result do case $1 in quote) func_append func_quote_portable_result "$3$2" set quote "$_G_part" "\\$_G_char" ;; start) set first "" "" func_quote_portable_result= ;; first) set quote "$_G_part" "" ;; esac done done IFS=$func_quote_portable_old_IFS ;; *) ;; esac break done func_quote_portable_unquoted_result=$func_quote_portable_result case $func_quote_portable_result in # double-quote args containing shell metacharacters to delay # word splitting, command substitution and variable expansion # for a subsequent eval. # many bourne shells cannot handle close brackets correctly # in scan sets, so we specify it separately. *[\[\~\#\^\&\*\(\)\{\}\|\;\<\>\?\'\ \ ]*|*]*|"") func_quote_portable_result=\"$func_quote_portable_result\" ;; esac } # func_quotefast_eval ARG # ----------------------- # Quote one ARG (internal). This is equivalent to 'func_quote_arg eval ARG', # but optimized for speed. Result is stored in $func_quotefast_eval. if test xyes = `(x=; printf -v x %q yes; echo x"$x") 2>/dev/null`; then printf -v _GL_test_printf_tilde %q '~' if test '\~' = "$_GL_test_printf_tilde"; then func_quotefast_eval () { printf -v func_quotefast_eval_result %q "$1" } else # Broken older Bash implementations. Make those faster too if possible. func_quotefast_eval () { case $1 in '~'*) func_quote_portable false "$1" func_quotefast_eval_result=$func_quote_portable_result ;; *) printf -v func_quotefast_eval_result %q "$1" ;; esac } fi else func_quotefast_eval () { func_quote_portable false "$1" func_quotefast_eval_result=$func_quote_portable_result } fi # func_quote_arg MODEs ARG # ------------------------ # Quote one ARG to be evaled later. MODEs argument may contain zero or more # specifiers listed below separated by ',' character. This function returns two # values: # i) func_quote_arg_result # double-quoted (when needed), suitable for a subsequent eval # ii) func_quote_arg_unquoted_result # has all characters that are still active within double # quotes backslashified. Available only if 'unquoted' is specified. # # Available modes: # ---------------- # 'eval' (default) # - escape shell special characters # 'expand' # - the same as 'eval'; but do not quote variable references # 'pretty' # - request aesthetic output, i.e. '"a b"' instead of 'a\ b'. This might # be used later in func_quote to get output like: 'echo "a b"' instead # of 'echo a\ b'. This is slower than default on some shells. # 'unquoted' # - produce also $func_quote_arg_unquoted_result which does not contain # wrapping double-quotes. # # Examples for 'func_quote_arg pretty,unquoted string': # # string | *_result | *_unquoted_result # ------------+-----------------------+------------------- # " | \" | \" # a b | "a b" | a b # "a b" | "\"a b\"" | \"a b\" # * | "*" | * # z="${x-$y}" | "z=\"\${x-\$y}\"" | z=\"\${x-\$y}\" # # Examples for 'func_quote_arg pretty,unquoted,expand string': # # string | *_result | *_unquoted_result # --------------+---------------------+-------------------- # z="${x-$y}" | "z=\"${x-$y}\"" | z=\"${x-$y}\" func_quote_arg () { _G_quote_expand=false case ,$1, in *,expand,*) _G_quote_expand=: ;; esac case ,$1, in *,pretty,*|*,expand,*|*,unquoted,*) func_quote_portable $_G_quote_expand "$2" func_quote_arg_result=$func_quote_portable_result func_quote_arg_unquoted_result=$func_quote_portable_unquoted_result ;; *) # Faster quote-for-eval for some shells. func_quotefast_eval "$2" func_quote_arg_result=$func_quotefast_eval_result ;; esac } # func_quote MODEs ARGs... # ------------------------ # Quote all ARGs to be evaled later and join them into single command. See # func_quote_arg's description for more info. func_quote () { $debug_cmd _G_func_quote_mode=$1 ; shift func_quote_result= while test 0 -lt $#; do func_quote_arg "$_G_func_quote_mode" "$1" if test -n "$func_quote_result"; then func_append func_quote_result " $func_quote_arg_result" else func_append func_quote_result "$func_quote_arg_result" fi shift done } # func_stripname PREFIX SUFFIX NAME # --------------------------------- # strip PREFIX and SUFFIX from NAME, and store in func_stripname_result. # PREFIX and SUFFIX must not contain globbing or regex special # characters, hashes, percent signs, but SUFFIX may contain a leading # dot (in which case that matches only a dot). if test yes = "$_G_HAVE_XSI_OPS"; then eval 'func_stripname () { $debug_cmd # pdksh 5.2.14 does not do ${X%$Y} correctly if both X and Y are # positional parameters, so assign one to ordinary variable first. func_stripname_result=$3 func_stripname_result=${func_stripname_result#"$1"} func_stripname_result=${func_stripname_result%"$2"} }' else func_stripname () { $debug_cmd case $2 in .*) func_stripname_result=`$ECHO "$3" | $SED -e "s%^$1%%" -e "s%\\\\$2\$%%"`;; *) func_stripname_result=`$ECHO "$3" | $SED -e "s%^$1%%" -e "s%$2\$%%"`;; esac } fi # func_show_eval CMD [FAIL_EXP] # ----------------------------- # Unless opt_quiet is true, then output CMD. Then, if opt_dryrun is # not true, evaluate CMD. If the evaluation of CMD fails, and FAIL_EXP # is given, then evaluate it. func_show_eval () { $debug_cmd _G_cmd=$1 _G_fail_exp=${2-':'} func_quote_arg pretty,expand "$_G_cmd" eval "func_notquiet $func_quote_arg_result" $opt_dry_run || { eval "$_G_cmd" _G_status=$? if test 0 -ne "$_G_status"; then eval "(exit $_G_status); $_G_fail_exp" fi } } # func_show_eval_locale CMD [FAIL_EXP] # ------------------------------------ # Unless opt_quiet is true, then output CMD. Then, if opt_dryrun is # not true, evaluate CMD. If the evaluation of CMD fails, and FAIL_EXP # is given, then evaluate it. Use the saved locale for evaluation. func_show_eval_locale () { $debug_cmd _G_cmd=$1 _G_fail_exp=${2-':'} $opt_quiet || { func_quote_arg expand,pretty "$_G_cmd" eval "func_echo $func_quote_arg_result" } $opt_dry_run || { eval "$_G_user_locale $_G_cmd" _G_status=$? eval "$_G_safe_locale" if test 0 -ne "$_G_status"; then eval "(exit $_G_status); $_G_fail_exp" fi } } # func_tr_sh # ---------- # Turn $1 into a string suitable for a shell variable name. # Result is stored in $func_tr_sh_result. All characters # not in the set a-zA-Z0-9_ are replaced with '_'. Further, # if $1 begins with a digit, a '_' is prepended as well. func_tr_sh () { $debug_cmd case $1 in [0-9]* | *[!a-zA-Z0-9_]*) func_tr_sh_result=`$ECHO "$1" | $SED -e 's/^\([0-9]\)/_\1/' -e 's/[^a-zA-Z0-9_]/_/g'` ;; * ) func_tr_sh_result=$1 ;; esac } # func_verbose ARG... # ------------------- # Echo program name prefixed message in verbose mode only. func_verbose () { $debug_cmd $opt_verbose && func_echo "$*" : } # func_warn_and_continue ARG... # ----------------------------- # Echo program name prefixed warning message to standard error. func_warn_and_continue () { $debug_cmd $require_term_colors func_echo_infix_1 "${tc_red}warning$tc_reset" "$*" >&2 } # func_warning CATEGORY ARG... # ---------------------------- # Echo program name prefixed warning message to standard error. Warning # messages can be filtered according to CATEGORY, where this function # elides messages where CATEGORY is not listed in the global variable # 'opt_warning_types'. func_warning () { $debug_cmd # CATEGORY must be in the warning_categories list! case " $warning_categories " in *" $1 "*) ;; *) func_internal_error "invalid warning category '$1'" ;; esac _G_category=$1 shift case " $opt_warning_types " in *" $_G_category "*) $warning_func ${1+"$@"} ;; esac } # func_sort_ver VER1 VER2 # ----------------------- # 'sort -V' is not generally available. # Note this deviates from the version comparison in automake # in that it treats 1.5 < 1.5.0, and treats 1.4.4a < 1.4-p3a # but this should suffice as we won't be specifying old # version formats or redundant trailing .0 in bootstrap.conf. # If we did want full compatibility then we should probably # use m4_version_compare from autoconf. func_sort_ver () { $debug_cmd printf '%s\n%s\n' "$1" "$2" \ | sort -t. -k 1,1n -k 2,2n -k 3,3n -k 4,4n -k 5,5n -k 6,6n -k 7,7n -k 8,8n -k 9,9n } # func_lt_ver PREV CURR # --------------------- # Return true if PREV and CURR are in the correct order according to # func_sort_ver, otherwise false. Use it like this: # # func_lt_ver "$prev_ver" "$proposed_ver" || func_fatal_error "..." func_lt_ver () { $debug_cmd test "x$1" = x`func_sort_ver "$1" "$2" | $SED 1q` } # Local variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'before-save-hook 'time-stamp) # time-stamp-pattern: "10/scriptversion=%:y-%02m-%02d.%02H; # UTC" # time-stamp-time-zone: "UTC" # End: #! /bin/sh # A portable, pluggable option parser for Bourne shell. # Written by Gary V. Vaughan, 2010 # This is free software. There is NO warranty; not even for # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. # # Copyright (C) 2010-2017 Bootstrap Authors # # This file is dual licensed under the terms of the MIT license # <https://opensource.org/license/MIT>, and GPL version 3 or later # <http://www.gnu.org/licenses/gpl-2.0.html>. You must apply one of # these licenses when using or redistributing this software or any of # the files within it. See the URLs above, or the file `LICENSE` # included in the Bootstrap distribution for the full license texts. # Please report bugs or propose patches to: # <https://github.com/gnulib-modules/bootstrap/issues> # Set a version string for this script. scriptversion=2016-03-06.01; # UTC ## ------ ## ## Usage. ## ## ------ ## # This file is a library for parsing options in your shell scripts along # with assorted other useful supporting features that you can make use # of too. # # For the simplest scripts you might need only: # # #!/bin/sh # . relative/path/to/funclib.sh # . relative/path/to/options-parser # scriptversion=1.0 # func_options ${1+"$@"} # eval set dummy "$func_options_result"; shift # ...rest of your script... # # In order for the '--version' option to work, you will need to have a # suitably formatted comment like the one at the top of this file # starting with '# Written by ' and ending with '# Copyright'. # # For '-h' and '--help' to work, you will also need a one line # description of your script's purpose in a comment directly above the # '# Written by ' line, like the one at the top of this file. # # The default options also support '--debug', which will turn on shell # execution tracing (see the comment above debug_cmd below for another # use), and '--verbose' and the func_verbose function to allow your script # to display verbose messages only when your user has specified # '--verbose'. # # After sourcing this file, you can plug in processing for additional # options by amending the variables from the 'Configuration' section # below, and following the instructions in the 'Option parsing' # section further down. ## -------------- ## ## Configuration. ## ## -------------- ## # You should override these variables in your script after sourcing this # file so that they reflect the customisations you have added to the # option parser. # The usage line for option parsing errors and the start of '-h' and # '--help' output messages. You can embed shell variables for delayed # expansion at the time the message is displayed, but you will need to # quote other shell meta-characters carefully to prevent them being # expanded when the contents are evaled. usage='$progpath [OPTION]...' # Short help message in response to '-h' and '--help'. Add to this or # override it after sourcing this library to reflect the full set of # options your script accepts. usage_message="\ --debug enable verbose shell tracing -W, --warnings=CATEGORY report the warnings falling in CATEGORY [all] -v, --verbose verbosely report processing --version print version information and exit -h, --help print short or long help message and exit " # Additional text appended to 'usage_message' in response to '--help'. long_help_message=" Warning categories include: 'all' show all warnings 'none' turn off all the warnings 'error' warnings are treated as fatal errors" # Help message printed before fatal option parsing errors. fatal_help="Try '\$progname --help' for more information." ## ------------------------- ## ## Hook function management. ## ## ------------------------- ## # This section contains functions for adding, removing, and running hooks # in the main code. A hook is just a list of function names that can be # run in order later on. # func_hookable FUNC_NAME # ----------------------- # Declare that FUNC_NAME will run hooks added with # 'func_add_hook FUNC_NAME ...'. func_hookable () { $debug_cmd func_append hookable_fns " $1" } # func_add_hook FUNC_NAME HOOK_FUNC # --------------------------------- # Request that FUNC_NAME call HOOK_FUNC before it returns. FUNC_NAME must # first have been declared "hookable" by a call to 'func_hookable'. func_add_hook () { $debug_cmd case " $hookable_fns " in *" $1 "*) ;; *) func_fatal_error "'$1' does not accept hook functions." ;; esac eval func_append ${1}_hooks '" $2"' } # func_remove_hook FUNC_NAME HOOK_FUNC # ------------------------------------ # Remove HOOK_FUNC from the list of hook functions to be called by # FUNC_NAME. func_remove_hook () { $debug_cmd eval ${1}_hooks='`$ECHO "\$'$1'_hooks" |$SED "s| '$2'||"`' } # func_propagate_result FUNC_NAME_A FUNC_NAME_B # --------------------------------------------- # If the *_result variable of FUNC_NAME_A _is set_, assign its value to # *_result variable of FUNC_NAME_B. func_propagate_result () { $debug_cmd func_propagate_result_result=: if eval "test \"\${${1}_result+set}\" = set" then eval "${2}_result=\$${1}_result" else func_propagate_result_result=false fi } # func_run_hooks FUNC_NAME [ARG]... # --------------------------------- # Run all hook functions registered to FUNC_NAME. # It's assumed that the list of hook functions contains nothing more # than a whitespace-delimited list of legal shell function names, and # no effort is wasted trying to catch shell meta-characters or preserve # whitespace. func_run_hooks () { $debug_cmd case " $hookable_fns " in *" $1 "*) ;; *) func_fatal_error "'$1' does not support hook functions." ;; esac eval _G_hook_fns=\$$1_hooks; shift for _G_hook in $_G_hook_fns; do func_unset "${_G_hook}_result" eval $_G_hook '${1+"$@"}' func_propagate_result $_G_hook func_run_hooks if $func_propagate_result_result; then eval set dummy "$func_run_hooks_result"; shift fi done } ## --------------- ## ## Option parsing. ## ## --------------- ## # In order to add your own option parsing hooks, you must accept the # full positional parameter list from your hook function. You may remove # or edit any options that you action, and then pass back the remaining # unprocessed options in '<hooked_function_name>_result', escaped # suitably for 'eval'. # # The '<hooked_function_name>_result' variable is automatically unset # before your hook gets called; for best performance, only set the # *_result variable when necessary (i.e. don't call the 'func_quote' # function unnecessarily because it can be an expensive operation on some # machines). # # Like this: # # my_options_prep () # { # $debug_cmd # # # Extend the existing usage message. # usage_message=$usage_message' # -s, --silent don'\''t print informational messages # ' # # No change in '$@' (ignored completely by this hook). Leave # # my_options_prep_result variable intact. # } # func_add_hook func_options_prep my_options_prep # # # my_silent_option () # { # $debug_cmd # # args_changed=false # # # Note that, for efficiency, we parse as many options as we can # # recognise in a loop before passing the remainder back to the # # caller on the first unrecognised argument we encounter. # while test $# -gt 0; do # opt=$1; shift # case $opt in # --silent|-s) opt_silent=: # args_changed=: # ;; # # Separate non-argument short options: # -s*) func_split_short_opt "$_G_opt" # set dummy "$func_split_short_opt_name" \ # "-$func_split_short_opt_arg" ${1+"$@"} # shift # args_changed=: # ;; # *) # Make sure the first unrecognised option "$_G_opt" # # is added back to "$@" in case we need it later, # # if $args_changed was set to 'true'. # set dummy "$_G_opt" ${1+"$@"}; shift; break ;; # esac # done # # # Only call 'func_quote' here if we processed at least one argument. # if $args_changed; then # func_quote eval ${1+"$@"} # my_silent_option_result=$func_quote_result # fi # } # func_add_hook func_parse_options my_silent_option # # # my_option_validation () # { # $debug_cmd # # $opt_silent && $opt_verbose && func_fatal_help "\ # '--silent' and '--verbose' options are mutually exclusive." # } # func_add_hook func_validate_options my_option_validation # # You'll also need to manually amend $usage_message to reflect the extra # options you parse. It's preferable to append if you can, so that # multiple option parsing hooks can be added safely. # func_options_finish [ARG]... # ---------------------------- # Finishing the option parse loop (call 'func_options' hooks ATM). func_options_finish () { $debug_cmd func_run_hooks func_options ${1+"$@"} func_propagate_result func_run_hooks func_options_finish } # func_options [ARG]... # --------------------- # All the functions called inside func_options are hookable. See the # individual implementations for details. func_hookable func_options func_options () { $debug_cmd _G_options_quoted=false for my_func in options_prep parse_options validate_options options_finish do func_unset func_${my_func}_result func_unset func_run_hooks_result eval func_$my_func '${1+"$@"}' func_propagate_result func_$my_func func_options if $func_propagate_result_result; then eval set dummy "$func_options_result"; shift _G_options_quoted=: fi done $_G_options_quoted || { # As we (func_options) are top-level options-parser function and # nobody quoted "$@" for us yet, we need to do it explicitly for # caller. func_quote eval ${1+"$@"} func_options_result=$func_quote_result } } # func_options_prep [ARG]... # -------------------------- # All initialisations required before starting the option parse loop. # Note that when calling hook functions, we pass through the list of # positional parameters. If a hook function modifies that list, and # needs to propagate that back to rest of this script, then the complete # modified list must be put in 'func_run_hooks_result' before returning. func_hookable func_options_prep func_options_prep () { $debug_cmd # Option defaults: opt_verbose=false opt_warning_types= func_run_hooks func_options_prep ${1+"$@"} func_propagate_result func_run_hooks func_options_prep } # func_parse_options [ARG]... # --------------------------- # The main option parsing loop. func_hookable func_parse_options func_parse_options () { $debug_cmd _G_parse_options_requote=false # this just eases exit handling while test $# -gt 0; do # Defer to hook functions for initial option parsing, so they # get priority in the event of reusing an option name. func_run_hooks func_parse_options ${1+"$@"} func_propagate_result func_run_hooks func_parse_options if $func_propagate_result_result; then eval set dummy "$func_parse_options_result"; shift # Even though we may have changed "$@", we passed the "$@" array # down into the hook and it quoted it for us (because we are in # this if-branch). No need to quote it again. _G_parse_options_requote=false fi # Break out of the loop if we already parsed every option. test $# -gt 0 || break # We expect that one of the options parsed in this function matches # and thus we remove _G_opt from "$@" and need to re-quote. _G_match_parse_options=: _G_opt=$1 shift case $_G_opt in --debug|-x) debug_cmd='set -x' func_echo "enabling shell trace mode" >&2 $debug_cmd ;; --no-warnings|--no-warning|--no-warn) set dummy --warnings none ${1+"$@"} shift ;; --warnings|--warning|-W) if test $# = 0 && func_missing_arg $_G_opt; then _G_parse_options_requote=: break fi case " $warning_categories $1" in *" $1 "*) # trailing space prevents matching last $1 above func_append_uniq opt_warning_types " $1" ;; *all) opt_warning_types=$warning_categories ;; *none) opt_warning_types=none warning_func=: ;; *error) opt_warning_types=$warning_categories warning_func=func_fatal_error ;; *) func_fatal_error \ "unsupported warning category: '$1'" ;; esac shift ;; --verbose|-v) opt_verbose=: ;; --version) func_version ;; -\?|-h) func_usage ;; --help) func_help ;; # Separate optargs to long options (plugins may need this): --*=*) func_split_equals "$_G_opt" set dummy "$func_split_equals_lhs" \ "$func_split_equals_rhs" ${1+"$@"} shift ;; # Separate optargs to short options: -W*) func_split_short_opt "$_G_opt" set dummy "$func_split_short_opt_name" \ "$func_split_short_opt_arg" ${1+"$@"} shift ;; # Separate non-argument short options: -\?*|-h*|-v*|-x*) func_split_short_opt "$_G_opt" set dummy "$func_split_short_opt_name" \ "-$func_split_short_opt_arg" ${1+"$@"} shift ;; --) _G_parse_options_requote=: ; break ;; -*) func_fatal_help "unrecognised option: '$_G_opt'" ;; *) set dummy "$_G_opt" ${1+"$@"}; shift _G_match_parse_options=false break ;; esac if $_G_match_parse_options; then _G_parse_options_requote=: fi done if $_G_parse_options_requote; then # save modified positional parameters for caller func_quote eval ${1+"$@"} func_parse_options_result=$func_quote_result fi } # func_validate_options [ARG]... # ------------------------------ # Perform any sanity checks on option settings and/or unconsumed # arguments. func_hookable func_validate_options func_validate_options () { $debug_cmd # Display all warnings if -W was not given. test -n "$opt_warning_types" || opt_warning_types=" $warning_categories" func_run_hooks func_validate_options ${1+"$@"} func_propagate_result func_run_hooks func_validate_options # Bail if the options were screwed! $exit_cmd $EXIT_FAILURE } ## ----------------- ## ## Helper functions. ## ## ----------------- ## # This section contains the helper functions used by the rest of the # hookable option parser framework in ascii-betical order. # func_fatal_help ARG... # ---------------------- # Echo program name prefixed message to standard error, followed by # a help hint, and exit. func_fatal_help () { $debug_cmd eval \$ECHO \""Usage: $usage"\" eval \$ECHO \""$fatal_help"\" func_error ${1+"$@"} exit $EXIT_FAILURE } # func_help # --------- # Echo long help message to standard output and exit. func_help () { $debug_cmd func_usage_message $ECHO "$long_help_message" exit 0 } # func_missing_arg ARGNAME # ------------------------ # Echo program name prefixed message to standard error and set global # exit_cmd. func_missing_arg () { $debug_cmd func_error "Missing argument for '$1'." exit_cmd=exit } # func_split_equals STRING # ------------------------ # Set func_split_equals_lhs and func_split_equals_rhs shell variables # after splitting STRING at the '=' sign. test -z "$_G_HAVE_XSI_OPS" \ && (eval 'x=a/b/c; test 5aa/bb/cc = "${#x}${x%%/*}${x%/*}${x#*/}${x##*/}"') 2>/dev/null \ && _G_HAVE_XSI_OPS=yes if test yes = "$_G_HAVE_XSI_OPS" then # This is an XSI compatible shell, allowing a faster implementation... eval 'func_split_equals () { $debug_cmd func_split_equals_lhs=${1%%=*} func_split_equals_rhs=${1#*=} if test "x$func_split_equals_lhs" = "x$1"; then func_split_equals_rhs= fi }' else # ...otherwise fall back to using expr, which is often a shell builtin. func_split_equals () { $debug_cmd func_split_equals_lhs=`expr "x$1" : 'x\([^=]*\)'` func_split_equals_rhs= test "x$func_split_equals_lhs" = "x$1" \ || func_split_equals_rhs=`expr "x$1" : 'x[^=]*=\(.*\)$'` } fi #func_split_equals # func_split_short_opt SHORTOPT # ----------------------------- # Set func_split_short_opt_name and func_split_short_opt_arg shell # variables after splitting SHORTOPT after the 2nd character. if test yes = "$_G_HAVE_XSI_OPS" then # This is an XSI compatible shell, allowing a faster implementation... eval 'func_split_short_opt () { $debug_cmd func_split_short_opt_arg=${1#??} func_split_short_opt_name=${1%"$func_split_short_opt_arg"} }' else # ...otherwise fall back to using expr, which is often a shell builtin. func_split_short_opt () { $debug_cmd func_split_short_opt_name=`expr "x$1" : 'x-\(.\)'` func_split_short_opt_arg=`expr "x$1" : 'x-.\(.*\)$'` } fi #func_split_short_opt # func_usage # ---------- # Echo short help message to standard output and exit. func_usage () { $debug_cmd func_usage_message $ECHO "Run '$progname --help |${PAGER-more}' for full usage" exit 0 } # func_usage_message # ------------------ # Echo short help message to standard output. func_usage_message () { $debug_cmd eval \$ECHO \""Usage: $usage"\" echo $SED -n 's|^# || /^Written by/{ x;p;x } h /^Written by/q' < "$progpath" echo eval \$ECHO \""$usage_message"\" } # func_version # ------------ # Echo version message to standard output and exit. # The version message is extracted from the calling file's header # comments, with leading '# ' stripped: # 1. First display the progname and version # 2. Followed by the header comment line matching /^# Written by / # 3. Then a blank line followed by the first following line matching # /^# Copyright / # 4. Immediately followed by any lines between the previous matches, # except lines preceding the intervening completely blank line. # For example, see the header comments of this file. func_version () { $debug_cmd printf '%s\n' "$progname $scriptversion" $SED -n ' /^# Written by /!b s|^# ||; p; n :fwd2blnk /./ { n b fwd2blnk } p; n :holdwrnt s|^# || s|^# *$|| /^Copyright /!{ /./H n b holdwrnt } s|\((C)\)[ 0-9,-]*[ ,-]\([1-9][0-9]* \)|\1 \2| G s|\(\n\)\n*|\1|g p; q' < "$progpath" exit $? } # Local variables: # mode: shell-script # sh-indentation: 2 # eval: (add-hook 'before-save-hook 'time-stamp) # time-stamp-pattern: "10/scriptversion=%:y-%02m-%02d.%02H; # UTC" # time-stamp-time-zone: "UTC" # End: # Set a version string. scriptversion='(GNU libtool) 2.4.6.40-6ca5-dirty' # func_echo ARG... # ---------------- # Libtool also displays the current mode in messages, so override # funclib.sh func_echo with this custom definition. func_echo () { $debug_cmd _G_message=$* func_echo_IFS=$IFS IFS=$nl for _G_line in $_G_message; do IFS=$func_echo_IFS $ECHO "$progname${opt_mode+: $opt_mode}: $_G_line" done IFS=$func_echo_IFS } # func_warning ARG... # ------------------- # Libtool warnings are not categorized, so override funclib.sh # func_warning with this simpler definition. func_warning () { $debug_cmd $warning_func ${1+"$@"} } ## ---------------- ## ## Options parsing. ## ## ---------------- ## # Hook in the functions to make sure our own options are parsed during # the option parsing loop. usage='$progpath [OPTION]... [MODE-ARG]...' # Short help message in response to '-h'. usage_message="Options: --config show all configuration variables --debug enable verbose shell tracing -n, --dry-run display commands without modifying any files --features display basic configuration information and exit --mode=MODE use operation mode MODE --no-warnings equivalent to '-Wnone' --preserve-dup-deps don't remove duplicate dependency libraries --quiet, --silent don't print informational messages --tag=TAG use configuration variables from tag TAG -v, --verbose print more informational messages than default --version print version information -W, --warnings=CATEGORY report the warnings falling in CATEGORY [all] -h, --help, --help-all print short, long, or detailed help message " # Additional text appended to 'usage_message' in response to '--help'. func_help () { $debug_cmd func_usage_message $ECHO "$long_help_message MODE must be one of the following: clean remove files from the build directory compile compile a source file into a libtool object execute automatically set library path, then run a program finish complete the installation of libtool libraries install install libraries or executables link create a library or an executable uninstall remove libraries from an installed directory MODE-ARGS vary depending on the MODE. When passed as first option, '--mode=MODE' may be abbreviated as 'MODE' or a unique abbreviation of that. Try '$progname --help --mode=MODE' for a more detailed description of MODE. When reporting a bug, please describe a test case to reproduce it and include the following information: host-triplet: $host shell: $SHELL compiler: $LTCC compiler flags: $LTCFLAGS linker: $LD (gnu? $with_gnu_ld) version: $progname (GNU libtool) 2.4.6.40-6ca5-dirty automake: `($AUTOMAKE --version) 2>/dev/null |$SED 1q` autoconf: `($AUTOCONF --version) 2>/dev/null |$SED 1q` Report bugs to <bug-libtool@gnu.org>. GNU libtool home page: <http://www.gnu.org/s/libtool/>. General help using GNU software: <http://www.gnu.org/gethelp/>." exit 0 } # func_lo2o OBJECT-NAME # --------------------- # Transform OBJECT-NAME from a '.lo' suffix to the platform specific # object suffix. lo2o=s/\\.lo\$/.$objext/ o2lo=s/\\.$objext\$/.lo/ if test yes = "$_G_HAVE_XSI_OPS"; then eval 'func_lo2o () { case $1 in *.lo) func_lo2o_result=${1%.lo}.$objext ;; * ) func_lo2o_result=$1 ;; esac }' # func_xform LIBOBJ-OR-SOURCE # --------------------------- # Transform LIBOBJ-OR-SOURCE from a '.o' or '.c' (or otherwise) # suffix to a '.lo' libtool-object suffix. eval 'func_xform () { func_xform_result=${1%.*}.lo }' else # ...otherwise fall back to using sed. func_lo2o () { func_lo2o_result=`$ECHO "$1" | $SED "$lo2o"` } func_xform () { func_xform_result=`$ECHO "$1" | $SED 's|\.[^.]*$|.lo|'` } fi # func_fatal_configuration ARG... # ------------------------------- # Echo program name prefixed message to standard error, followed by # a configuration failure hint, and exit. func_fatal_configuration () { func_fatal_error ${1+"$@"} \ "See the $PACKAGE documentation for more information." \ "Fatal configuration error." } # func_config # ----------- # Display the configuration for all the tags in this script. func_config () { re_begincf='^# ### BEGIN LIBTOOL' re_endcf='^# ### END LIBTOOL' # Default configuration. $SED "1,/$re_begincf CONFIG/d;/$re_endcf CONFIG/,\$d" < "$progpath" # Now print the configurations for the tags. for tagname in $taglist; do $SED -n "/$re_begincf TAG CONFIG: $tagname\$/,/$re_endcf TAG CONFIG: $tagname\$/p" < "$progpath" done exit $? } # func_features # ------------- # Display the features supported by this script. func_features () { echo "host: $host" if test yes = "$build_libtool_libs"; then echo "enable shared libraries" else echo "disable shared libraries" fi if test yes = "$build_old_libs"; then echo "enable static libraries" else echo "disable static libraries" fi exit $? } # func_enable_tag TAGNAME # ----------------------- # Verify that TAGNAME is valid, and either flag an error and exit, or # enable the TAGNAME tag. We also add TAGNAME to the global $taglist # variable here. func_enable_tag () { # Global variable: tagname=$1 re_begincf="^# ### BEGIN LIBTOOL TAG CONFIG: $tagname\$" re_endcf="^# ### END LIBTOOL TAG CONFIG: $tagname\$" sed_extractcf=/$re_begincf/,/$re_endcf/p # Validate tagname. case $tagname in *[!-_A-Za-z0-9,/]*) func_fatal_error "invalid tag name: $tagname" ;; esac # Don't test for the "default" C tag, as we know it's # there but not specially marked. case $tagname in CC) ;; *) if $GREP "$re_begincf" "$progpath" >/dev/null 2>&1; then taglist="$taglist $tagname" # Evaluate the configuration. Be careful to quote the path # and the sed script, to avoid splitting on whitespace, but # also don't use non-portable quotes within backquotes within # quotes we have to do it in 2 steps: extractedcf=`$SED -n -e "$sed_extractcf" < "$progpath"` eval "$extractedcf" else func_error "ignoring unknown tag $tagname" fi ;; esac } # func_check_version_match # ------------------------ # Ensure that we are using m4 macros, and libtool script from the same # release of libtool. func_check_version_match () { if test "$package_revision" != "$macro_revision"; then if test "$VERSION" != "$macro_version"; then if test -z "$macro_version"; then cat >&2 <<_LT_EOF $progname: Version mismatch error. This is $PACKAGE $VERSION, but the $progname: definition of this LT_INIT comes from an older release. $progname: You should recreate aclocal.m4 with macros from $PACKAGE $VERSION $progname: and run autoconf again. _LT_EOF else cat >&2 <<_LT_EOF $progname: Version mismatch error. This is $PACKAGE $VERSION, but the $progname: definition of this LT_INIT comes from $PACKAGE $macro_version. $progname: You should recreate aclocal.m4 with macros from $PACKAGE $VERSION $progname: and run autoconf again. _LT_EOF fi else cat >&2 <<_LT_EOF $progname: Version mismatch error. This is $PACKAGE $VERSION, revision $package_revision, $progname: but the definition of this LT_INIT comes from revision $macro_revision. $progname: You should recreate aclocal.m4 with macros from revision $package_revision $progname: of $PACKAGE $VERSION and run autoconf again. _LT_EOF fi exit $EXIT_MISMATCH fi } # libtool_options_prep [ARG]... # ----------------------------- # Preparation for options parsed by libtool. libtool_options_prep () { $debug_mode # Option defaults: opt_config=false opt_dlopen= opt_dry_run=false opt_help=false opt_mode= opt_preserve_dup_deps=false opt_quiet=false nonopt= preserve_args= _G_rc_lt_options_prep=: # Shorthand for --mode=foo, only valid as the first argument case $1 in clean|clea|cle|cl) shift; set dummy --mode clean ${1+"$@"}; shift ;; compile|compil|compi|comp|com|co|c) shift; set dummy --mode compile ${1+"$@"}; shift ;; execute|execut|execu|exec|exe|ex|e) shift; set dummy --mode execute ${1+"$@"}; shift ;; finish|finis|fini|fin|fi|f) shift; set dummy --mode finish ${1+"$@"}; shift ;; install|instal|insta|inst|ins|in|i) shift; set dummy --mode install ${1+"$@"}; shift ;; link|lin|li|l) shift; set dummy --mode link ${1+"$@"}; shift ;; uninstall|uninstal|uninsta|uninst|unins|unin|uni|un|u) shift; set dummy --mode uninstall ${1+"$@"}; shift ;; *) _G_rc_lt_options_prep=false ;; esac if $_G_rc_lt_options_prep; then # Pass back the list of options. func_quote eval ${1+"$@"} libtool_options_prep_result=$func_quote_result fi } func_add_hook func_options_prep libtool_options_prep # libtool_parse_options [ARG]... # --------------------------------- # Provide handling for libtool specific options. libtool_parse_options () { $debug_cmd _G_rc_lt_parse_options=false # Perform our own loop to consume as many options as possible in # each iteration. while test $# -gt 0; do _G_match_lt_parse_options=: _G_opt=$1 shift case $_G_opt in --dry-run|--dryrun|-n) opt_dry_run=: ;; --config) func_config ;; --dlopen|-dlopen) opt_dlopen="${opt_dlopen+$opt_dlopen }$1" shift ;; --preserve-dup-deps) opt_preserve_dup_deps=: ;; --features) func_features ;; --finish) set dummy --mode finish ${1+"$@"}; shift ;; --help) opt_help=: ;; --help-all) opt_help=': help-all' ;; --mode) test $# = 0 && func_missing_arg $_G_opt && break opt_mode=$1 case $1 in # Valid mode arguments: clean|compile|execute|finish|install|link|relink|uninstall) ;; # Catch anything else as an error *) func_error "invalid argument for $_G_opt" exit_cmd=exit break ;; esac shift ;; --no-silent|--no-quiet) opt_quiet=false func_append preserve_args " $_G_opt" ;; --no-warnings|--no-warning|--no-warn) opt_warning=false func_append preserve_args " $_G_opt" ;; --no-verbose) opt_verbose=false func_append preserve_args " $_G_opt" ;; --silent|--quiet) opt_quiet=: opt_verbose=false func_append preserve_args " $_G_opt" ;; --tag) test $# = 0 && func_missing_arg $_G_opt && break opt_tag=$1 func_append preserve_args " $_G_opt $1" func_enable_tag "$1" shift ;; --verbose|-v) opt_quiet=false opt_verbose=: func_append preserve_args " $_G_opt" ;; # An option not handled by this hook function: *) set dummy "$_G_opt" ${1+"$@"} ; shift _G_match_lt_parse_options=false break ;; esac $_G_match_lt_parse_options && _G_rc_lt_parse_options=: done if $_G_rc_lt_parse_options; then # save modified positional parameters for caller func_quote eval ${1+"$@"} libtool_parse_options_result=$func_quote_result fi } func_add_hook func_parse_options libtool_parse_options # libtool_validate_options [ARG]... # --------------------------------- # Perform any sanity checks on option settings and/or unconsumed # arguments. libtool_validate_options () { # save first non-option argument if test 0 -lt $#; then nonopt=$1 shift fi # preserve --debug test : = "$debug_cmd" || func_append preserve_args " --debug" case $host in # Solaris2 added to fix http://debbugs.gnu.org/cgi/bugreport.cgi?bug=16452 # see also: http://gcc.gnu.org/bugzilla/show_bug.cgi?id=59788 *cygwin* | *mingw* | *pw32* | *cegcc* | *solaris2* | *os2*) # don't eliminate duplications in $postdeps and $predeps opt_duplicate_compiler_generated_deps=: ;; *) opt_duplicate_compiler_generated_deps=$opt_preserve_dup_deps ;; esac $opt_help || { # Sanity checks first: func_check_version_match test yes != "$build_libtool_libs" \ && test yes != "$build_old_libs" \ && func_fatal_configuration "not configured to build any kind of library" # Darwin sucks eval std_shrext=\"$shrext_cmds\" # Only execute mode is allowed to have -dlopen flags. if test -n "$opt_dlopen" && test execute != "$opt_mode"; then func_error "unrecognized option '-dlopen'" $ECHO "$help" 1>&2 exit $EXIT_FAILURE fi # Change the help message to a mode-specific one. generic_help=$help help="Try '$progname --help --mode=$opt_mode' for more information." } # Pass back the unparsed argument list func_quote eval ${1+"$@"} libtool_validate_options_result=$func_quote_result } func_add_hook func_validate_options libtool_validate_options # Process options as early as possible so that --help and --version # can return quickly. func_options ${1+"$@"} eval set dummy "$func_options_result"; shift ## ----------- ## ## Main. ## ## ----------- ## magic='%%%MAGIC variable%%%' magic_exe='%%%MAGIC EXE variable%%%' # Global variables. extracted_archives= extracted_serial=0 # If this variable is set in any of the actions, the command in it # will be execed at the end. This prevents here-documents from being # left over by shells. exec_cmd= # A function that is used when there is no print builtin or printf. func_fallback_echo () { eval 'cat <<_LTECHO_EOF $1 _LTECHO_EOF' } # func_generated_by_libtool # True iff stdin has been generated by Libtool. This function is only # a basic sanity check; it will hardly flush out determined imposters. func_generated_by_libtool_p () { $GREP "^# Generated by .*$PACKAGE" > /dev/null 2>&1 } # func_lalib_p file # True iff FILE is a libtool '.la' library or '.lo' object file. # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_lalib_p () { test -f "$1" && $SED -e 4q "$1" 2>/dev/null | func_generated_by_libtool_p } # func_lalib_unsafe_p file # True iff FILE is a libtool '.la' library or '.lo' object file. # This function implements the same check as func_lalib_p without # resorting to external programs. To this end, it redirects stdin and # closes it afterwards, without saving the original file descriptor. # As a safety measure, use it only where a negative result would be # fatal anyway. Works if 'file' does not exist. func_lalib_unsafe_p () { lalib_p=no if test -f "$1" && test -r "$1" && exec 5<&0 <"$1"; then for lalib_p_l in 1 2 3 4 do read lalib_p_line case $lalib_p_line in \#\ Generated\ by\ *$PACKAGE* ) lalib_p=yes; break;; esac done exec 0<&5 5<&- fi test yes = "$lalib_p" } # func_ltwrapper_script_p file # True iff FILE is a libtool wrapper script # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_ltwrapper_script_p () { test -f "$1" && $lt_truncate_bin < "$1" 2>/dev/null | func_generated_by_libtool_p } # func_ltwrapper_executable_p file # True iff FILE is a libtool wrapper executable # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_ltwrapper_executable_p () { func_ltwrapper_exec_suffix= case $1 in *.exe) ;; *) func_ltwrapper_exec_suffix=.exe ;; esac $GREP "$magic_exe" "$1$func_ltwrapper_exec_suffix" >/dev/null 2>&1 } # func_ltwrapper_scriptname file # Assumes file is an ltwrapper_executable # uses $file to determine the appropriate filename for a # temporary ltwrapper_script. func_ltwrapper_scriptname () { func_dirname_and_basename "$1" "" "." func_stripname '' '.exe' "$func_basename_result" func_ltwrapper_scriptname_result=$func_dirname_result/$objdir/${func_stripname_result}_ltshwrapper } # func_ltwrapper_p file # True iff FILE is a libtool wrapper script or wrapper executable # This function is only a basic sanity check; it will hardly flush out # determined imposters. func_ltwrapper_p () { func_ltwrapper_script_p "$1" || func_ltwrapper_executable_p "$1" } # func_execute_cmds commands fail_cmd # Execute tilde-delimited COMMANDS. # If FAIL_CMD is given, eval that upon failure. # FAIL_CMD may read-access the current command in variable CMD! func_execute_cmds () { $debug_cmd save_ifs=$IFS; IFS='~' for cmd in $1; do IFS=$sp$nl eval cmd=\"$cmd\" IFS=$save_ifs func_show_eval "$cmd" "${2-:}" done IFS=$save_ifs } # func_source file # Source FILE, adding directory component if necessary. # Note that it is not necessary on cygwin/mingw to append a dot to # FILE even if both FILE and FILE.exe exist: automatic-append-.exe # behavior happens only for exec(3), not for open(2)! Also, sourcing # 'FILE.' does not work on cygwin managed mounts. func_source () { $debug_cmd case $1 in */* | *\\*) . "$1" ;; *) . "./$1" ;; esac } # func_resolve_sysroot PATH # Replace a leading = in PATH with a sysroot. Store the result into # func_resolve_sysroot_result func_resolve_sysroot () { func_resolve_sysroot_result=$1 case $func_resolve_sysroot_result in =*) func_stripname '=' '' "$func_resolve_sysroot_result" func_resolve_sysroot_result=$lt_sysroot$func_stripname_result ;; esac } # func_replace_sysroot PATH # If PATH begins with the sysroot, replace it with = and # store the result into func_replace_sysroot_result. func_replace_sysroot () { case $lt_sysroot:$1 in ?*:"$lt_sysroot"*) func_stripname "$lt_sysroot" '' "$1" func_replace_sysroot_result='='$func_stripname_result ;; *) # Including no sysroot. func_replace_sysroot_result=$1 ;; esac } # func_infer_tag arg # Infer tagged configuration to use if any are available and # if one wasn't chosen via the "--tag" command line option. # Only attempt this if the compiler in the base compile # command doesn't match the default compiler. # arg is usually of the form 'gcc ...' func_infer_tag () { $debug_cmd if test -n "$available_tags" && test -z "$tagname"; then CC_quoted= for arg in $CC; do func_append_quoted CC_quoted "$arg" done CC_expanded=`func_echo_all $CC` CC_quoted_expanded=`func_echo_all $CC_quoted` case $@ in # Blanks in the command may have been stripped by the calling shell, # but not from the CC environment variable when configure was run. " $CC "* | "$CC "* | " $CC_expanded "* | "$CC_expanded "* | \ " $CC_quoted"* | "$CC_quoted "* | " $CC_quoted_expanded "* | "$CC_quoted_expanded "*) ;; # Blanks at the start of $base_compile will cause this to fail # if we don't check for them as well. *) for z in $available_tags; do if $GREP "^# ### BEGIN LIBTOOL TAG CONFIG: $z$" < "$progpath" > /dev/null; then # Evaluate the configuration. eval "`$SED -n -e '/^# ### BEGIN LIBTOOL TAG CONFIG: '$z'$/,/^# ### END LIBTOOL TAG CONFIG: '$z'$/p' < $progpath`" CC_quoted= for arg in $CC; do # Double-quote args containing other shell metacharacters. func_append_quoted CC_quoted "$arg" done CC_expanded=`func_echo_all $CC` CC_quoted_expanded=`func_echo_all $CC_quoted` case "$@ " in " $CC "* | "$CC "* | " $CC_expanded "* | "$CC_expanded "* | \ " $CC_quoted"* | "$CC_quoted "* | " $CC_quoted_expanded "* | "$CC_quoted_expanded "*) # The compiler in the base compile command matches # the one in the tagged configuration. # Assume this is the tagged configuration we want. tagname=$z break ;; esac fi done # If $tagname still isn't set, then no tagged configuration # was found and let the user know that the "--tag" command # line option must be used. if test -z "$tagname"; then func_echo "unable to infer tagged configuration" func_fatal_error "specify a tag with '--tag'" # else # func_verbose "using $tagname tagged configuration" fi ;; esac fi } # func_write_libtool_object output_name pic_name nonpic_name # Create a libtool object file (analogous to a ".la" file), # but don't create it if we're doing a dry run. func_write_libtool_object () { write_libobj=$1 if test yes = "$build_libtool_libs"; then write_lobj=\'$2\' else write_lobj=none fi if test yes = "$build_old_libs"; then write_oldobj=\'$3\' else write_oldobj=none fi $opt_dry_run || { cat >${write_libobj}T <<EOF # $write_libobj - a libtool object file # Generated by $PROGRAM (GNU $PACKAGE) $VERSION # # Please DO NOT delete this file! # It is necessary for linking the library. # Name of the PIC object. pic_object=$write_lobj # Name of the non-PIC object non_pic_object=$write_oldobj EOF $MV "${write_libobj}T" "$write_libobj" } } ################################################## # FILE NAME AND PATH CONVERSION HELPER FUNCTIONS # ################################################## # func_convert_core_file_wine_to_w32 ARG # Helper function used by file name conversion functions when $build is *nix, # and $host is mingw, cygwin, or some other w32 environment. Relies on a # correctly configured wine environment available, with the winepath program # in $build's $PATH. # # ARG is the $build file name to be converted to w32 format. # Result is available in $func_convert_core_file_wine_to_w32_result, and will # be empty on error (or when ARG is empty) func_convert_core_file_wine_to_w32 () { $debug_cmd func_convert_core_file_wine_to_w32_result=$1 if test -n "$1"; then # Unfortunately, winepath does not exit with a non-zero error code, so we # are forced to check the contents of stdout. On the other hand, if the # command is not found, the shell will set an exit code of 127 and print # *an error message* to stdout. So we must check for both error code of # zero AND non-empty stdout, which explains the odd construction: func_convert_core_file_wine_to_w32_tmp=`winepath -w "$1" 2>/dev/null` if test "$?" -eq 0 && test -n "$func_convert_core_file_wine_to_w32_tmp"; then func_convert_core_file_wine_to_w32_result=`$ECHO "$func_convert_core_file_wine_to_w32_tmp" | $SED -e "$sed_naive_backslashify"` else func_convert_core_file_wine_to_w32_result= fi fi } # end: func_convert_core_file_wine_to_w32 # func_convert_core_path_wine_to_w32 ARG # Helper function used by path conversion functions when $build is *nix, and # $host is mingw, cygwin, or some other w32 environment. Relies on a correctly # configured wine environment available, with the winepath program in $build's # $PATH. Assumes ARG has no leading or trailing path separator characters. # # ARG is path to be converted from $build format to win32. # Result is available in $func_convert_core_path_wine_to_w32_result. # Unconvertible file (directory) names in ARG are skipped; if no directory names # are convertible, then the result may be empty. func_convert_core_path_wine_to_w32 () { $debug_cmd # unfortunately, winepath doesn't convert paths, only file names func_convert_core_path_wine_to_w32_result= if test -n "$1"; then oldIFS=$IFS IFS=: for func_convert_core_path_wine_to_w32_f in $1; do IFS=$oldIFS func_convert_core_file_wine_to_w32 "$func_convert_core_path_wine_to_w32_f" if test -n "$func_convert_core_file_wine_to_w32_result"; then if test -z "$func_convert_core_path_wine_to_w32_result"; then func_convert_core_path_wine_to_w32_result=$func_convert_core_file_wine_to_w32_result else func_append func_convert_core_path_wine_to_w32_result ";$func_convert_core_file_wine_to_w32_result" fi fi done IFS=$oldIFS fi } # end: func_convert_core_path_wine_to_w32 # func_cygpath ARGS... # Wrapper around calling the cygpath program via LT_CYGPATH. This is used when # when (1) $build is *nix and Cygwin is hosted via a wine environment; or (2) # $build is MSYS and $host is Cygwin, or (3) $build is Cygwin. In case (1) or # (2), returns the Cygwin file name or path in func_cygpath_result (input # file name or path is assumed to be in w32 format, as previously converted # from $build's *nix or MSYS format). In case (3), returns the w32 file name # or path in func_cygpath_result (input file name or path is assumed to be in # Cygwin format). Returns an empty string on error. # # ARGS are passed to cygpath, with the last one being the file name or path to # be converted. # # Specify the absolute *nix (or w32) name to cygpath in the LT_CYGPATH # environment variable; do not put it in $PATH. func_cygpath () { $debug_cmd if test -n "$LT_CYGPATH" && test -f "$LT_CYGPATH"; then func_cygpath_result=`$LT_CYGPATH "$@" 2>/dev/null` if test "$?" -ne 0; then # on failure, ensure result is empty func_cygpath_result= fi else func_cygpath_result= func_error "LT_CYGPATH is empty or specifies non-existent file: '$LT_CYGPATH'" fi } #end: func_cygpath # func_convert_core_msys_to_w32 ARG # Convert file name or path ARG from MSYS format to w32 format. Return # result in func_convert_core_msys_to_w32_result. func_convert_core_msys_to_w32 () { $debug_cmd # awkward: cmd appends spaces to result func_convert_core_msys_to_w32_result=`( cmd //c echo "$1" ) 2>/dev/null | $SED -e 's/[ ]*$//' -e "$sed_naive_backslashify"` } #end: func_convert_core_msys_to_w32 # func_convert_file_check ARG1 ARG2 # Verify that ARG1 (a file name in $build format) was converted to $host # format in ARG2. Otherwise, emit an error message, but continue (resetting # func_to_host_file_result to ARG1). func_convert_file_check () { $debug_cmd if test -z "$2" && test -n "$1"; then func_error "Could not determine host file name corresponding to" func_error " '$1'" func_error "Continuing, but uninstalled executables may not work." # Fallback: func_to_host_file_result=$1 fi } # end func_convert_file_check # func_convert_path_check FROM_PATHSEP TO_PATHSEP FROM_PATH TO_PATH # Verify that FROM_PATH (a path in $build format) was converted to $host # format in TO_PATH. Otherwise, emit an error message, but continue, resetting # func_to_host_file_result to a simplistic fallback value (see below). func_convert_path_check () { $debug_cmd if test -z "$4" && test -n "$3"; then func_error "Could not determine the host path corresponding to" func_error " '$3'" func_error "Continuing, but uninstalled executables may not work." # Fallback. This is a deliberately simplistic "conversion" and # should not be "improved". See libtool.info. if test "x$1" != "x$2"; then lt_replace_pathsep_chars="s|$1|$2|g" func_to_host_path_result=`echo "$3" | $SED -e "$lt_replace_pathsep_chars"` else func_to_host_path_result=$3 fi fi } # end func_convert_path_check # func_convert_path_front_back_pathsep FRONTPAT BACKPAT REPL ORIG # Modifies func_to_host_path_result by prepending REPL if ORIG matches FRONTPAT # and appending REPL if ORIG matches BACKPAT. func_convert_path_front_back_pathsep () { $debug_cmd case $4 in $1 ) func_to_host_path_result=$3$func_to_host_path_result ;; esac case $4 in $2 ) func_append func_to_host_path_result "$3" ;; esac } # end func_convert_path_front_back_pathsep ################################################## # $build to $host FILE NAME CONVERSION FUNCTIONS # ################################################## # invoked via '$to_host_file_cmd ARG' # # In each case, ARG is the path to be converted from $build to $host format. # Result will be available in $func_to_host_file_result. # func_to_host_file ARG # Converts the file name ARG from $build format to $host format. Return result # in func_to_host_file_result. func_to_host_file () { $debug_cmd $to_host_file_cmd "$1" } # end func_to_host_file # func_to_tool_file ARG LAZY # converts the file name ARG from $build format to toolchain format. Return # result in func_to_tool_file_result. If the conversion in use is listed # in (the comma separated) LAZY, no conversion takes place. func_to_tool_file () { $debug_cmd case ,$2, in *,"$to_tool_file_cmd",*) func_to_tool_file_result=$1 ;; *) $to_tool_file_cmd "$1" func_to_tool_file_result=$func_to_host_file_result ;; esac } # end func_to_tool_file # func_convert_file_noop ARG # Copy ARG to func_to_host_file_result. func_convert_file_noop () { func_to_host_file_result=$1 } # end func_convert_file_noop # func_convert_file_msys_to_w32 ARG # Convert file name ARG from (mingw) MSYS to (mingw) w32 format; automatic # conversion to w32 is not available inside the cwrapper. Returns result in # func_to_host_file_result. func_convert_file_msys_to_w32 () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then func_convert_core_msys_to_w32 "$1" func_to_host_file_result=$func_convert_core_msys_to_w32_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_msys_to_w32 # func_convert_file_cygwin_to_w32 ARG # Convert file name ARG from Cygwin to w32 format. Returns result in # func_to_host_file_result. func_convert_file_cygwin_to_w32 () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then # because $build is cygwin, we call "the" cygpath in $PATH; no need to use # LT_CYGPATH in this case. func_to_host_file_result=`cygpath -m "$1"` fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_cygwin_to_w32 # func_convert_file_nix_to_w32 ARG # Convert file name ARG from *nix to w32 format. Requires a wine environment # and a working winepath. Returns result in func_to_host_file_result. func_convert_file_nix_to_w32 () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then func_convert_core_file_wine_to_w32 "$1" func_to_host_file_result=$func_convert_core_file_wine_to_w32_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_nix_to_w32 # func_convert_file_msys_to_cygwin ARG # Convert file name ARG from MSYS to Cygwin format. Requires LT_CYGPATH set. # Returns result in func_to_host_file_result. func_convert_file_msys_to_cygwin () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then func_convert_core_msys_to_w32 "$1" func_cygpath -u "$func_convert_core_msys_to_w32_result" func_to_host_file_result=$func_cygpath_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_msys_to_cygwin # func_convert_file_nix_to_cygwin ARG # Convert file name ARG from *nix to Cygwin format. Requires Cygwin installed # in a wine environment, working winepath, and LT_CYGPATH set. Returns result # in func_to_host_file_result. func_convert_file_nix_to_cygwin () { $debug_cmd func_to_host_file_result=$1 if test -n "$1"; then # convert from *nix to w32, then use cygpath to convert from w32 to cygwin. func_convert_core_file_wine_to_w32 "$1" func_cygpath -u "$func_convert_core_file_wine_to_w32_result" func_to_host_file_result=$func_cygpath_result fi func_convert_file_check "$1" "$func_to_host_file_result" } # end func_convert_file_nix_to_cygwin ############################################# # $build to $host PATH CONVERSION FUNCTIONS # ############################################# # invoked via '$to_host_path_cmd ARG' # # In each case, ARG is the path to be converted from $build to $host format. # The result will be available in $func_to_host_path_result. # # Path separators are also converted from $build format to $host format. If # ARG begins or ends with a path separator character, it is preserved (but # converted to $host format) on output. # # All path conversion functions are named using the following convention: # file name conversion function : func_convert_file_X_to_Y () # path conversion function : func_convert_path_X_to_Y () # where, for any given $build/$host combination the 'X_to_Y' value is the # same. If conversion functions are added for new $build/$host combinations, # the two new functions must follow this pattern, or func_init_to_host_path_cmd # will break. # func_init_to_host_path_cmd # Ensures that function "pointer" variable $to_host_path_cmd is set to the # appropriate value, based on the value of $to_host_file_cmd. to_host_path_cmd= func_init_to_host_path_cmd () { $debug_cmd if test -z "$to_host_path_cmd"; then func_stripname 'func_convert_file_' '' "$to_host_file_cmd" to_host_path_cmd=func_convert_path_$func_stripname_result fi } # func_to_host_path ARG # Converts the path ARG from $build format to $host format. Return result # in func_to_host_path_result. func_to_host_path () { $debug_cmd func_init_to_host_path_cmd $to_host_path_cmd "$1" } # end func_to_host_path # func_convert_path_noop ARG # Copy ARG to func_to_host_path_result. func_convert_path_noop () { func_to_host_path_result=$1 } # end func_convert_path_noop # func_convert_path_msys_to_w32 ARG # Convert path ARG from (mingw) MSYS to (mingw) w32 format; automatic # conversion to w32 is not available inside the cwrapper. Returns result in # func_to_host_path_result. func_convert_path_msys_to_w32 () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # Remove leading and trailing path separator characters from ARG. MSYS # behavior is inconsistent here; cygpath turns them into '.;' and ';.'; # and winepath ignores them completely. func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_msys_to_w32 "$func_to_host_path_tmp1" func_to_host_path_result=$func_convert_core_msys_to_w32_result func_convert_path_check : ";" \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" ";" "$1" fi } # end func_convert_path_msys_to_w32 # func_convert_path_cygwin_to_w32 ARG # Convert path ARG from Cygwin to w32 format. Returns result in # func_to_host_file_result. func_convert_path_cygwin_to_w32 () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # See func_convert_path_msys_to_w32: func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_to_host_path_result=`cygpath -m -p "$func_to_host_path_tmp1"` func_convert_path_check : ";" \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" ";" "$1" fi } # end func_convert_path_cygwin_to_w32 # func_convert_path_nix_to_w32 ARG # Convert path ARG from *nix to w32 format. Requires a wine environment and # a working winepath. Returns result in func_to_host_file_result. func_convert_path_nix_to_w32 () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # See func_convert_path_msys_to_w32: func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_path_wine_to_w32 "$func_to_host_path_tmp1" func_to_host_path_result=$func_convert_core_path_wine_to_w32_result func_convert_path_check : ";" \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" ";" "$1" fi } # end func_convert_path_nix_to_w32 # func_convert_path_msys_to_cygwin ARG # Convert path ARG from MSYS to Cygwin format. Requires LT_CYGPATH set. # Returns result in func_to_host_file_result. func_convert_path_msys_to_cygwin () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # See func_convert_path_msys_to_w32: func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_msys_to_w32 "$func_to_host_path_tmp1" func_cygpath -u -p "$func_convert_core_msys_to_w32_result" func_to_host_path_result=$func_cygpath_result func_convert_path_check : : \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" : "$1" fi } # end func_convert_path_msys_to_cygwin # func_convert_path_nix_to_cygwin ARG # Convert path ARG from *nix to Cygwin format. Requires Cygwin installed in a # a wine environment, working winepath, and LT_CYGPATH set. Returns result in # func_to_host_file_result. func_convert_path_nix_to_cygwin () { $debug_cmd func_to_host_path_result=$1 if test -n "$1"; then # Remove leading and trailing path separator characters from # ARG. msys behavior is inconsistent here, cygpath turns them # into '.;' and ';.', and winepath ignores them completely. func_stripname : : "$1" func_to_host_path_tmp1=$func_stripname_result func_convert_core_path_wine_to_w32 "$func_to_host_path_tmp1" func_cygpath -u -p "$func_convert_core_path_wine_to_w32_result" func_to_host_path_result=$func_cygpath_result func_convert_path_check : : \ "$func_to_host_path_tmp1" "$func_to_host_path_result" func_convert_path_front_back_pathsep ":*" "*:" : "$1" fi } # end func_convert_path_nix_to_cygwin # func_dll_def_p FILE # True iff FILE is a Windows DLL '.def' file. # Keep in sync with _LT_DLL_DEF_P in libtool.m4 func_dll_def_p () { $debug_cmd func_dll_def_p_tmp=`$SED -n \ -e 's/^[ ]*//' \ -e '/^\(;.*\)*$/d' \ -e 's/^\(EXPORTS\|LIBRARY\)\([ ].*\)*$/DEF/p' \ -e q \ "$1"` test DEF = "$func_dll_def_p_tmp" } # func_mode_compile arg... func_mode_compile () { $debug_cmd # Get the compilation command and the source file. base_compile= srcfile=$nonopt # always keep a non-empty value in "srcfile" suppress_opt=yes suppress_output= arg_mode=normal libobj= later= pie_flag= for arg do case $arg_mode in arg ) # do not "continue". Instead, add this to base_compile lastarg=$arg arg_mode=normal ;; target ) libobj=$arg arg_mode=normal continue ;; normal ) # Accept any command-line options. case $arg in -o) test -n "$libobj" && \ func_fatal_error "you cannot specify '-o' more than once" arg_mode=target continue ;; -pie | -fpie | -fPIE) func_append pie_flag " $arg" continue ;; -shared | -static | -prefer-pic | -prefer-non-pic) func_append later " $arg" continue ;; -no-suppress) suppress_opt=no continue ;; -Xcompiler) arg_mode=arg # the next one goes into the "base_compile" arg list continue # The current "srcfile" will either be retained or ;; # replaced later. I would guess that would be a bug. -Wc,*) func_stripname '-Wc,' '' "$arg" args=$func_stripname_result lastarg= save_ifs=$IFS; IFS=, for arg in $args; do IFS=$save_ifs func_append_quoted lastarg "$arg" done IFS=$save_ifs func_stripname ' ' '' "$lastarg" lastarg=$func_stripname_result # Add the arguments to base_compile. func_append base_compile " $lastarg" continue ;; *) # Accept the current argument as the source file. # The previous "srcfile" becomes the current argument. # lastarg=$srcfile srcfile=$arg ;; esac # case $arg ;; esac # case $arg_mode # Aesthetically quote the previous argument. func_append_quoted base_compile "$lastarg" done # for arg case $arg_mode in arg) func_fatal_error "you must specify an argument for -Xcompile" ;; target) func_fatal_error "you must specify a target with '-o'" ;; *) # Get the name of the library object. test -z "$libobj" && { func_basename "$srcfile" libobj=$func_basename_result } ;; esac # Recognize several different file suffixes. # If the user specifies -o file.o, it is replaced with file.lo case $libobj in *.[cCFSifmso] | \ *.ada | *.adb | *.ads | *.asm | \ *.c++ | *.cc | *.ii | *.class | *.cpp | *.cxx | \ *.[fF][09]? | *.for | *.java | *.go | *.obj | *.sx | *.cu | *.cup) func_xform "$libobj" libobj=$func_xform_result ;; esac case $libobj in *.lo) func_lo2o "$libobj"; obj=$func_lo2o_result ;; *) func_fatal_error "cannot determine name of library object from '$libobj'" ;; esac func_infer_tag $base_compile for arg in $later; do case $arg in -shared) test yes = "$build_libtool_libs" \ || func_fatal_configuration "cannot build a shared library" build_old_libs=no continue ;; -static) build_libtool_libs=no build_old_libs=yes continue ;; -prefer-pic) pic_mode=yes continue ;; -prefer-non-pic) pic_mode=no continue ;; esac done func_quote_arg pretty "$libobj" test "X$libobj" != "X$func_quote_arg_result" \ && $ECHO "X$libobj" | $GREP '[]~#^*{};<>?"'"'"' &()|`$[]' \ && func_warning "libobj name '$libobj' may not contain shell special characters." func_dirname_and_basename "$obj" "/" "" objname=$func_basename_result xdir=$func_dirname_result lobj=$xdir$objdir/$objname test -z "$base_compile" && \ func_fatal_help "you must specify a compilation command" # Delete any leftover library objects. if test yes = "$build_old_libs"; then removelist="$obj $lobj $libobj ${libobj}T" else removelist="$lobj $libobj ${libobj}T" fi # On Cygwin there's no "real" PIC flag so we must build both object types case $host_os in cygwin* | mingw* | pw32* | os2* | cegcc*) pic_mode=default ;; esac if test no = "$pic_mode" && test pass_all != "$deplibs_check_method"; then # non-PIC code in shared libraries is not supported pic_mode=default fi # Calculate the filename of the output object if compiler does # not support -o with -c if test no = "$compiler_c_o"; then output_obj=`$ECHO "$srcfile" | $SED 's%^.*/%%; s%\.[^.]*$%%'`.$objext lockfile=$output_obj.lock else output_obj= need_locks=no lockfile= fi # Lock this critical section if it is needed # We use this script file to make the link, it avoids creating a new file if test yes = "$need_locks"; then until $opt_dry_run || ln "$progpath" "$lockfile" 2>/dev/null; do func_echo "Waiting for $lockfile to be removed" sleep 2 done elif test warn = "$need_locks"; then if test -f "$lockfile"; then $ECHO "\ *** ERROR, $lockfile exists and contains: `cat $lockfile 2>/dev/null` This indicates that another process is trying to use the same temporary object file, and libtool could not work around it because your compiler does not support '-c' and '-o' together. If you repeat this compilation, it may succeed, by chance, but you had better avoid parallel builds (make -j) in this platform, or get a better compiler." $opt_dry_run || $RM $removelist exit $EXIT_FAILURE fi func_append removelist " $output_obj" $ECHO "$srcfile" > "$lockfile" fi $opt_dry_run || $RM $removelist func_append removelist " $lockfile" trap '$opt_dry_run || $RM $removelist; exit $EXIT_FAILURE' 1 2 15 func_to_tool_file "$srcfile" func_convert_file_msys_to_w32 srcfile=$func_to_tool_file_result func_quote_arg pretty "$srcfile" qsrcfile=$func_quote_arg_result # Only build a PIC object if we are building libtool libraries. if test yes = "$build_libtool_libs"; then # Without this assignment, base_compile gets emptied. fbsd_hideous_sh_bug=$base_compile if test no != "$pic_mode"; then command="$base_compile $qsrcfile $pic_flag" else # Don't build PIC code command="$base_compile $qsrcfile" fi func_mkdir_p "$xdir$objdir" if test -z "$output_obj"; then # Place PIC objects in $objdir func_append command " -o $lobj" fi func_show_eval_locale "$command" \ 'test -n "$output_obj" && $RM $removelist; exit $EXIT_FAILURE' if test warn = "$need_locks" && test "X`cat $lockfile 2>/dev/null`" != "X$srcfile"; then $ECHO "\ *** ERROR, $lockfile contains: `cat $lockfile 2>/dev/null` but it should contain: $srcfile This indicates that another process is trying to use the same temporary object file, and libtool could not work around it because your compiler does not support '-c' and '-o' together. If you repeat this compilation, it may succeed, by chance, but you had better avoid parallel builds (make -j) in this platform, or get a better compiler." $opt_dry_run || $RM $removelist exit $EXIT_FAILURE fi # Just move the object if needed, then go on to compile the next one if test -n "$output_obj" && test "X$output_obj" != "X$lobj"; then func_show_eval '$MV "$output_obj" "$lobj"' \ 'error=$?; $opt_dry_run || $RM $removelist; exit $error' fi # Allow error messages only from the first compilation. if test yes = "$suppress_opt"; then suppress_output=' >/dev/null 2>&1' fi fi # Only build a position-dependent object if we build old libraries. if test yes = "$build_old_libs"; then if test yes != "$pic_mode"; then # Don't build PIC code command="$base_compile $qsrcfile$pie_flag" else command="$base_compile $qsrcfile $pic_flag" fi if test yes = "$compiler_c_o"; then func_append command " -o $obj" fi # Suppress compiler output if we already did a PIC compilation. func_append command "$suppress_output" func_show_eval_locale "$command" \ '$opt_dry_run || $RM $removelist; exit $EXIT_FAILURE' if test warn = "$need_locks" && test "X`cat $lockfile 2>/dev/null`" != "X$srcfile"; then $ECHO "\ *** ERROR, $lockfile contains: `cat $lockfile 2>/dev/null` but it should contain: $srcfile This indicates that another process is trying to use the same temporary object file, and libtool could not work around it because your compiler does not support '-c' and '-o' together. If you repeat this compilation, it may succeed, by chance, but you had better avoid parallel builds (make -j) in this platform, or get a better compiler." $opt_dry_run || $RM $removelist exit $EXIT_FAILURE fi # Just move the object if needed if test -n "$output_obj" && test "X$output_obj" != "X$obj"; then func_show_eval '$MV "$output_obj" "$obj"' \ 'error=$?; $opt_dry_run || $RM $removelist; exit $error' fi fi $opt_dry_run || { func_write_libtool_object "$libobj" "$objdir/$objname" "$objname" # Unlock the critical section if it was locked if test no != "$need_locks"; then removelist=$lockfile $RM "$lockfile" fi } exit $EXIT_SUCCESS } $opt_help || { test compile = "$opt_mode" && func_mode_compile ${1+"$@"} } func_mode_help () { # We need to display help for each of the modes. case $opt_mode in "") # Generic help is extracted from the usage comments # at the start of this file. func_help ;; clean) $ECHO \ "Usage: $progname [OPTION]... --mode=clean RM [RM-OPTION]... FILE... Remove files from the build directory. RM is the name of the program to use to delete files associated with each FILE (typically '/bin/rm'). RM-OPTIONS are options (such as '-f') to be passed to RM. If FILE is a libtool library, object or program, all the files associated with it are deleted. Otherwise, only FILE itself is deleted using RM." ;; compile) $ECHO \ "Usage: $progname [OPTION]... --mode=compile COMPILE-COMMAND... SOURCEFILE Compile a source file into a libtool library object. This mode accepts the following additional options: -o OUTPUT-FILE set the output file name to OUTPUT-FILE -no-suppress do not suppress compiler output for multiple passes -prefer-pic try to build PIC objects only -prefer-non-pic try to build non-PIC objects only -shared do not build a '.o' file suitable for static linking -static only build a '.o' file suitable for static linking -Wc,FLAG pass FLAG directly to the compiler COMPILE-COMMAND is a command to be used in creating a 'standard' object file from the given SOURCEFILE. The output file name is determined by removing the directory component from SOURCEFILE, then substituting the C source code suffix '.c' with the library object suffix, '.lo'." ;; execute) $ECHO \ "Usage: $progname [OPTION]... --mode=execute COMMAND [ARGS]... Automatically set library path, then run a program. This mode accepts the following additional options: -dlopen FILE add the directory containing FILE to the library path This mode sets the library path environment variable according to '-dlopen' flags. If any of the ARGS are libtool executable wrappers, then they are translated into their corresponding uninstalled binary, and any of their required library directories are added to the library path. Then, COMMAND is executed, with ARGS as arguments." ;; finish) $ECHO \ "Usage: $progname [OPTION]... --mode=finish [LIBDIR]... Complete the installation of libtool libraries. Each LIBDIR is a directory that contains libtool libraries. The commands that this mode executes may require superuser privileges. Use the '--dry-run' option if you just want to see what would be executed." ;; install) $ECHO \ "Usage: $progname [OPTION]... --mode=install INSTALL-COMMAND... Install executables or libraries. INSTALL-COMMAND is the installation command. The first component should be either the 'install' or 'cp' program. The following components of INSTALL-COMMAND are treated specially: -inst-prefix-dir PREFIX-DIR Use PREFIX-DIR as a staging area for installation The rest of the components are interpreted as arguments to that command (only BSD-compatible install options are recognized)." ;; link) $ECHO \ "Usage: $progname [OPTION]... --mode=link LINK-COMMAND... Link object files or libraries together to form another library, or to create an executable program. LINK-COMMAND is a command using the C compiler that you would use to create a program from several object files. The following components of LINK-COMMAND are treated specially: -all-static do not do any dynamic linking at all -avoid-version do not add a version suffix if possible -bindir BINDIR specify path to binaries directory (for systems where libraries must be found in the PATH setting at runtime) -dlopen FILE '-dlpreopen' FILE if it cannot be dlopened at runtime -dlpreopen FILE link in FILE and add its symbols to lt_preloaded_symbols -export-dynamic allow symbols from OUTPUT-FILE to be resolved with dlsym(3) -export-symbols SYMFILE try to export only the symbols listed in SYMFILE -export-symbols-regex REGEX try to export only the symbols matching REGEX -LLIBDIR search LIBDIR for required installed libraries -lNAME OUTPUT-FILE requires the installed library libNAME -module build a library that can dlopened -no-fast-install disable the fast-install mode -no-install link a not-installable executable -no-undefined declare that a library does not refer to external symbols -o OUTPUT-FILE create OUTPUT-FILE from the specified objects -objectlist FILE use a list of object files found in FILE to specify objects -os2dllname NAME force a short DLL name on OS/2 (no effect on other OSes) -precious-files-regex REGEX don't remove output files matching REGEX -release RELEASE specify package release information -rpath LIBDIR the created library will eventually be installed in LIBDIR -R[ ]LIBDIR add LIBDIR to the runtime path of programs and libraries -shared only do dynamic linking of libtool libraries -shrext SUFFIX override the standard shared library file extension -static do not do any dynamic linking of uninstalled libtool libraries -static-libtool-libs do not do any dynamic linking of libtool libraries -version-info CURRENT[:REVISION[:AGE]] specify library version info [each variable defaults to 0] -weak LIBNAME declare that the target provides the LIBNAME interface -Wc,FLAG -Xcompiler FLAG pass linker-specific FLAG directly to the compiler -Wl,FLAG -Xlinker FLAG pass linker-specific FLAG directly to the linker -XCClinker FLAG pass link-specific FLAG to the compiler driver (CC) All other options (arguments beginning with '-') are ignored. Every other argument is treated as a filename. Files ending in '.la' are treated as uninstalled libtool libraries, other files are standard or library object files. If the OUTPUT-FILE ends in '.la', then a libtool library is created, only library objects ('.lo' files) may be specified, and '-rpath' is required, except when creating a convenience library. If OUTPUT-FILE ends in '.a' or '.lib', then a standard library is created using 'ar' and 'ranlib', or on Windows using 'lib'. If OUTPUT-FILE ends in '.lo' or '.$objext', then a reloadable object file is created, otherwise an executable program is created." ;; uninstall) $ECHO \ "Usage: $progname [OPTION]... --mode=uninstall RM [RM-OPTION]... FILE... Remove libraries from an installation directory. RM is the name of the program to use to delete files associated with each FILE (typically '/bin/rm'). RM-OPTIONS are options (such as '-f') to be passed to RM. If FILE is a libtool library, all the files associated with it are deleted. Otherwise, only FILE itself is deleted using RM." ;; *) func_fatal_help "invalid operation mode '$opt_mode'" ;; esac echo $ECHO "Try '$progname --help' for more information about other modes." } # Now that we've collected a possible --mode arg, show help if necessary if $opt_help; then if test : = "$opt_help"; then func_mode_help else { func_help noexit for opt_mode in compile link execute install finish uninstall clean; do func_mode_help done } | $SED -n '1p; 2,$s/^Usage:/ or: /p' { func_help noexit for opt_mode in compile link execute install finish uninstall clean; do echo func_mode_help done } | $SED '1d /^When reporting/,/^Report/{ H d } $x /information about other modes/d /more detailed .*MODE/d s/^Usage:.*--mode=\([^ ]*\) .*/Description of \1 mode:/' fi exit $? fi # func_mode_execute arg... func_mode_execute () { $debug_cmd # The first argument is the command name. cmd=$nonopt test -z "$cmd" && \ func_fatal_help "you must specify a COMMAND" # Handle -dlopen flags immediately. for file in $opt_dlopen; do test -f "$file" \ || func_fatal_help "'$file' is not a file" dir= case $file in *.la) func_resolve_sysroot "$file" file=$func_resolve_sysroot_result # Check to see that this really is a libtool archive. func_lalib_unsafe_p "$file" \ || func_fatal_help "'$lib' is not a valid libtool archive" # Read the libtool library. dlname= library_names= func_source "$file" # Skip this library if it cannot be dlopened. if test -z "$dlname"; then # Warn if it was a shared library. test -n "$library_names" && \ func_warning "'$file' was not linked with '-export-dynamic'" continue fi func_dirname "$file" "" "." dir=$func_dirname_result if test -f "$dir/$objdir/$dlname"; then func_append dir "/$objdir" else if test ! -f "$dir/$dlname"; then func_fatal_error "cannot find '$dlname' in '$dir' or '$dir/$objdir'" fi fi ;; *.lo) # Just add the directory containing the .lo file. func_dirname "$file" "" "." dir=$func_dirname_result ;; *) func_warning "'-dlopen' is ignored for non-libtool libraries and objects" continue ;; esac # Get the absolute pathname. absdir=`cd "$dir" && pwd` test -n "$absdir" && dir=$absdir # Now add the directory to shlibpath_var. if eval "test -z \"\$$shlibpath_var\""; then eval "$shlibpath_var=\"\$dir\"" else eval "$shlibpath_var=\"\$dir:\$$shlibpath_var\"" fi done # This variable tells wrapper scripts just to set shlibpath_var # rather than running their programs. libtool_execute_magic=$magic # Check if any of the arguments is a wrapper script. args= for file do case $file in -* | *.la | *.lo ) ;; *) # Do a test to see if this is really a libtool program. if func_ltwrapper_script_p "$file"; then func_source "$file" # Transform arg to wrapped name. file=$progdir/$program elif func_ltwrapper_executable_p "$file"; then func_ltwrapper_scriptname "$file" func_source "$func_ltwrapper_scriptname_result" # Transform arg to wrapped name. file=$progdir/$program fi ;; esac # Quote arguments (to preserve shell metacharacters). func_append_quoted args "$file" done if $opt_dry_run; then # Display what would be done. if test -n "$shlibpath_var"; then eval "\$ECHO \"\$shlibpath_var=\$$shlibpath_var\"" echo "export $shlibpath_var" fi $ECHO "$cmd$args" exit $EXIT_SUCCESS else if test -n "$shlibpath_var"; then # Export the shlibpath_var. eval "export $shlibpath_var" fi # Restore saved environment variables for lt_var in LANG LANGUAGE LC_ALL LC_CTYPE LC_COLLATE LC_MESSAGES do eval "if test \"\${save_$lt_var+set}\" = set; then $lt_var=\$save_$lt_var; export $lt_var else $lt_unset $lt_var fi" done # Now prepare to actually exec the command. exec_cmd=\$cmd$args fi } test execute = "$opt_mode" && func_mode_execute ${1+"$@"} # func_mode_finish arg... func_mode_finish () { $debug_cmd libs= libdirs= admincmds= for opt in "$nonopt" ${1+"$@"} do if test -d "$opt"; then func_append libdirs " $opt" elif test -f "$opt"; then if func_lalib_unsafe_p "$opt"; then func_append libs " $opt" else func_warning "'$opt' is not a valid libtool archive" fi else func_fatal_error "invalid argument '$opt'" fi done if test -n "$libs"; then if test -n "$lt_sysroot"; then sysroot_regex=`$ECHO "$lt_sysroot" | $SED "$sed_make_literal_regex"` sysroot_cmd="s/\([ ']\)$sysroot_regex/\1/g;" else sysroot_cmd= fi # Remove sysroot references if $opt_dry_run; then for lib in $libs; do echo "removing references to $lt_sysroot and '=' prefixes from $lib" done else tmpdir=`func_mktempdir` for lib in $libs; do $SED -e "$sysroot_cmd s/\([ ']-[LR]\)=/\1/g; s/\([ ']\)=/\1/g" $lib \ > $tmpdir/tmp-la mv -f $tmpdir/tmp-la $lib done ${RM}r "$tmpdir" fi fi if test -n "$finish_cmds$finish_eval" && test -n "$libdirs"; then for libdir in $libdirs; do if test -n "$finish_cmds"; then # Do each command in the finish commands. func_execute_cmds "$finish_cmds" 'admincmds="$admincmds '"$cmd"'"' fi if test -n "$finish_eval"; then # Do the single finish_eval. eval cmds=\"$finish_eval\" $opt_dry_run || eval "$cmds" || func_append admincmds " $cmds" fi done fi # Exit here if they wanted silent mode. $opt_quiet && exit $EXIT_SUCCESS if test -n "$finish_cmds$finish_eval" && test -n "$libdirs"; then echo "----------------------------------------------------------------------" echo "Libraries have been installed in:" for libdir in $libdirs; do $ECHO " $libdir" done echo echo "If you ever happen to want to link against installed libraries" echo "in a given directory, LIBDIR, you must either use libtool, and" echo "specify the full pathname of the library, or use the '-LLIBDIR'" echo "flag during linking and do at least one of the following:" if test -n "$shlibpath_var"; then echo " - add LIBDIR to the '$shlibpath_var' environment variable" echo " during execution" fi if test -n "$runpath_var"; then echo " - add LIBDIR to the '$runpath_var' environment variable" echo " during linking" fi if test -n "$hardcode_libdir_flag_spec"; then libdir=LIBDIR eval flag=\"$hardcode_libdir_flag_spec\" $ECHO " - use the '$flag' linker flag" fi if test -n "$admincmds"; then $ECHO " - have your system administrator run these commands:$admincmds" fi if test -f /etc/ld.so.conf; then echo " - have your system administrator add LIBDIR to '/etc/ld.so.conf'" fi echo echo "See any operating system documentation about shared libraries for" case $host in solaris2.[6789]|solaris2.1[0-9]) echo "more information, such as the ld(1), crle(1) and ld.so(8) manual" echo "pages." ;; *) echo "more information, such as the ld(1) and ld.so(8) manual pages." ;; esac echo "----------------------------------------------------------------------" fi exit $EXIT_SUCCESS } test finish = "$opt_mode" && func_mode_finish ${1+"$@"} # func_mode_install arg... func_mode_install () { $debug_cmd # There may be an optional sh(1) argument at the beginning of # install_prog (especially on Windows NT). if test "$SHELL" = "$nonopt" || test /bin/sh = "$nonopt" || # Allow the use of GNU shtool's install command. case $nonopt in *shtool*) :;; *) false;; esac then # Aesthetically quote it. func_quote_arg pretty "$nonopt" install_prog="$func_quote_arg_result " arg=$1 shift else install_prog= arg=$nonopt fi # The real first argument should be the name of the installation program. # Aesthetically quote it. func_quote_arg pretty "$arg" func_append install_prog "$func_quote_arg_result" install_shared_prog=$install_prog case " $install_prog " in *[\\\ /]cp\ *) install_cp=: ;; *) install_cp=false ;; esac # We need to accept at least all the BSD install flags. dest= files= opts= prev= install_type= isdir=false stripme= no_mode=: for arg do arg2= if test -n "$dest"; then func_append files " $dest" dest=$arg continue fi case $arg in -d) isdir=: ;; -f) if $install_cp; then :; else prev=$arg fi ;; -g | -m | -o) prev=$arg ;; -s) stripme=" -s" continue ;; -*) ;; *) # If the previous option needed an argument, then skip it. if test -n "$prev"; then if test X-m = "X$prev" && test -n "$install_override_mode"; then arg2=$install_override_mode no_mode=false fi prev= else dest=$arg continue fi ;; esac # Aesthetically quote the argument. func_quote_arg pretty "$arg" func_append install_prog " $func_quote_arg_result" if test -n "$arg2"; then func_quote_arg pretty "$arg2" fi func_append install_shared_prog " $func_quote_arg_result" done test -z "$install_prog" && \ func_fatal_help "you must specify an install program" test -n "$prev" && \ func_fatal_help "the '$prev' option requires an argument" if test -n "$install_override_mode" && $no_mode; then if $install_cp; then :; else func_quote_arg pretty "$install_override_mode" func_append install_shared_prog " -m $func_quote_arg_result" fi fi if test -z "$files"; then if test -z "$dest"; then func_fatal_help "no file or destination specified" else func_fatal_help "you must specify a destination" fi fi # Strip any trailing slash from the destination. func_stripname '' '/' "$dest" dest=$func_stripname_result # Check to see that the destination is a directory. test -d "$dest" && isdir=: if $isdir; then destdir=$dest destname= else func_dirname_and_basename "$dest" "" "." destdir=$func_dirname_result destname=$func_basename_result # Not a directory, so check to see that there is only one file specified. set dummy $files; shift test "$#" -gt 1 && \ func_fatal_help "'$dest' is not a directory" fi case $destdir in [\\/]* | [A-Za-z]:[\\/]*) ;; *) for file in $files; do case $file in *.lo) ;; *) func_fatal_help "'$destdir' must be an absolute directory name" ;; esac done ;; esac # This variable tells wrapper scripts just to set variables rather # than running their programs. libtool_install_magic=$magic staticlibs= future_libdirs= current_libdirs= for file in $files; do # Do each installation. case $file in *.$libext) # Do the static libraries later. func_append staticlibs " $file" ;; *.la) func_resolve_sysroot "$file" file=$func_resolve_sysroot_result # Check to see that this really is a libtool archive. func_lalib_unsafe_p "$file" \ || func_fatal_help "'$file' is not a valid libtool archive" library_names= old_library= relink_command= func_source "$file" # Add the libdir to current_libdirs if it is the destination. if test "X$destdir" = "X$libdir"; then case "$current_libdirs " in *" $libdir "*) ;; *) func_append current_libdirs " $libdir" ;; esac else # Note the libdir as a future libdir. case "$future_libdirs " in *" $libdir "*) ;; *) func_append future_libdirs " $libdir" ;; esac fi func_dirname "$file" "/" "" dir=$func_dirname_result func_append dir "$objdir" if test -n "$relink_command"; then # Determine the prefix the user has applied to our future dir. inst_prefix_dir=`$ECHO "$destdir" | $SED -e "s%$libdir\$%%"` # Don't allow the user to place us outside of our expected # location b/c this prevents finding dependent libraries that # are installed to the same prefix. # At present, this check doesn't affect windows .dll's that # are installed into $libdir/../bin (currently, that works fine) # but it's something to keep an eye on. test "$inst_prefix_dir" = "$destdir" && \ func_fatal_error "error: cannot install '$file' to a directory not ending in $libdir" if test -n "$inst_prefix_dir"; then # Stick the inst_prefix_dir data into the link command. relink_command=`$ECHO "$relink_command" | $SED "s%@inst_prefix_dir@%-inst-prefix-dir $inst_prefix_dir%"` else relink_command=`$ECHO "$relink_command" | $SED "s%@inst_prefix_dir@%%"` fi func_warning "relinking '$file'" func_show_eval "$relink_command" \ 'func_fatal_error "error: relink '\''$file'\'' with the above command before installing it"' fi # See the names of the shared library. set dummy $library_names; shift if test -n "$1"; then realname=$1 shift srcname=$realname test -n "$relink_command" && srcname=${realname}T # Install the shared library and build the symlinks. func_show_eval "$install_shared_prog $dir/$srcname $destdir/$realname" \ 'exit $?' tstripme=$stripme case $host_os in cygwin* | mingw* | pw32* | cegcc*) case $realname in *.dll.a) tstripme= ;; esac ;; os2*) case $realname in *_dll.a) tstripme= ;; esac ;; esac if test -n "$tstripme" && test -n "$striplib"; then func_show_eval "$striplib $destdir/$realname" 'exit $?' fi if test "$#" -gt 0; then # Delete the old symlinks, and create new ones. # Try 'ln -sf' first, because the 'ln' binary might depend on # the symlink we replace! Solaris /bin/ln does not understand -f, # so we also need to try rm && ln -s. for linkname do test "$linkname" != "$realname" \ && func_show_eval "(cd $destdir && { $LN_S -f $realname $linkname || { $RM $linkname && $LN_S $realname $linkname; }; })" done fi # Do each command in the postinstall commands. lib=$destdir/$realname func_execute_cmds "$postinstall_cmds" 'exit $?' fi # Install the pseudo-library for information purposes. func_basename "$file" name=$func_basename_result instname=$dir/${name}i func_show_eval "$install_prog $instname $destdir/$name" 'exit $?' # Maybe install the static library, too. test -n "$old_library" && func_append staticlibs " $dir/$old_library" ;; *.lo) # Install (i.e. copy) a libtool object. # Figure out destination file name, if it wasn't already specified. if test -n "$destname"; then destfile=$destdir/$destname else func_basename "$file" destfile=$func_basename_result destfile=$destdir/$destfile fi # Deduce the name of the destination old-style object file. case $destfile in *.lo) func_lo2o "$destfile" staticdest=$func_lo2o_result ;; *.$objext) staticdest=$destfile destfile= ;; *) func_fatal_help "cannot copy a libtool object to '$destfile'" ;; esac # Install the libtool object if requested. test -n "$destfile" && \ func_show_eval "$install_prog $file $destfile" 'exit $?' # Install the old object if enabled. if test yes = "$build_old_libs"; then # Deduce the name of the old-style object file. func_lo2o "$file" staticobj=$func_lo2o_result func_show_eval "$install_prog \$staticobj \$staticdest" 'exit $?' fi exit $EXIT_SUCCESS ;; *) # Figure out destination file name, if it wasn't already specified. if test -n "$destname"; then destfile=$destdir/$destname else func_basename "$file" destfile=$func_basename_result destfile=$destdir/$destfile fi # If the file is missing, and there is a .exe on the end, strip it # because it is most likely a libtool script we actually want to # install stripped_ext= case $file in *.exe) if test ! -f "$file"; then func_stripname '' '.exe' "$file" file=$func_stripname_result stripped_ext=.exe fi ;; esac # Do a test to see if this is really a libtool program. case $host in *cygwin* | *mingw*) if func_ltwrapper_executable_p "$file"; then func_ltwrapper_scriptname "$file" wrapper=$func_ltwrapper_scriptname_result else func_stripname '' '.exe' "$file" wrapper=$func_stripname_result fi ;; *) wrapper=$file ;; esac if func_ltwrapper_script_p "$wrapper"; then notinst_deplibs= relink_command= func_source "$wrapper" # Check the variables that should have been set. test -z "$generated_by_libtool_version" && \ func_fatal_error "invalid libtool wrapper script '$wrapper'" finalize=: for lib in $notinst_deplibs; do # Check to see that each library is installed. libdir= if test -f "$lib"; then func_source "$lib" fi libfile=$libdir/`$ECHO "$lib" | $SED 's%^.*/%%g'` if test -n "$libdir" && test ! -f "$libfile"; then func_warning "'$lib' has not been installed in '$libdir'" finalize=false fi done relink_command= func_source "$wrapper" outputname= if test no = "$fast_install" && test -n "$relink_command"; then $opt_dry_run || { if $finalize; then tmpdir=`func_mktempdir` func_basename "$file$stripped_ext" file=$func_basename_result outputname=$tmpdir/$file # Replace the output file specification. relink_command=`$ECHO "$relink_command" | $SED 's%@OUTPUT@%'"$outputname"'%g'` $opt_quiet || { func_quote_arg expand,pretty "$relink_command" eval "func_echo $func_quote_arg_result" } if eval "$relink_command"; then : else func_error "error: relink '$file' with the above command before installing it" $opt_dry_run || ${RM}r "$tmpdir" continue fi file=$outputname else func_warning "cannot relink '$file'" fi } else # Install the binary that we compiled earlier. file=`$ECHO "$file$stripped_ext" | $SED "s%\([^/]*\)$%$objdir/\1%"` fi fi # remove .exe since cygwin /usr/bin/install will append another # one anyway case $install_prog,$host in */usr/bin/install*,*cygwin*) case $file:$destfile in *.exe:*.exe) # this is ok ;; *.exe:*) destfile=$destfile.exe ;; *:*.exe) func_stripname '' '.exe' "$destfile" destfile=$func_stripname_result ;; esac ;; esac func_show_eval "$install_prog\$stripme \$file \$destfile" 'exit $?' $opt_dry_run || if test -n "$outputname"; then ${RM}r "$tmpdir" fi ;; esac done for file in $staticlibs; do func_basename "$file" name=$func_basename_result # Set up the ranlib parameters. oldlib=$destdir/$name func_to_tool_file "$oldlib" func_convert_file_msys_to_w32 tool_oldlib=$func_to_tool_file_result func_show_eval "$install_prog \$file \$oldlib" 'exit $?' if test -n "$stripme" && test -n "$old_striplib"; then func_show_eval "$old_striplib $tool_oldlib" 'exit $?' fi # Do each command in the postinstall commands. func_execute_cmds "$old_postinstall_cmds" 'exit $?' done test -n "$future_libdirs" && \ func_warning "remember to run '$progname --finish$future_libdirs'" if test -n "$current_libdirs"; then # Maybe just do a dry run. $opt_dry_run && current_libdirs=" -n$current_libdirs" exec_cmd='$SHELL "$progpath" $preserve_args --finish$current_libdirs' else exit $EXIT_SUCCESS fi } test install = "$opt_mode" && func_mode_install ${1+"$@"} # func_generate_dlsyms outputname originator pic_p # Extract symbols from dlprefiles and create ${outputname}S.o with # a dlpreopen symbol table. func_generate_dlsyms () { $debug_cmd my_outputname=$1 my_originator=$2 my_pic_p=${3-false} my_prefix=`$ECHO "$my_originator" | $SED 's%[^a-zA-Z0-9]%_%g'` my_dlsyms= if test -n "$dlfiles$dlprefiles" || test no != "$dlself"; then if test -n "$NM" && test -n "$global_symbol_pipe"; then my_dlsyms=${my_outputname}S.c else func_error "not configured to extract global symbols from dlpreopened files" fi fi if test -n "$my_dlsyms"; then case $my_dlsyms in "") ;; *.c) # Discover the nlist of each of the dlfiles. nlist=$output_objdir/$my_outputname.nm func_show_eval "$RM $nlist ${nlist}S ${nlist}T" # Parse the name list into a source file. func_verbose "creating $output_objdir/$my_dlsyms" $opt_dry_run || $ECHO > "$output_objdir/$my_dlsyms" "\ /* $my_dlsyms - symbol resolution table for '$my_outputname' dlsym emulation. */ /* Generated by $PROGRAM (GNU $PACKAGE) $VERSION */ #ifdef __cplusplus extern \"C\" { #endif #if defined __GNUC__ && (((__GNUC__ == 4) && (__GNUC_MINOR__ >= 4)) || (__GNUC__ > 4)) #pragma GCC diagnostic ignored \"-Wstrict-prototypes\" #endif /* Keep this code in sync between libtool.m4, ltmain, lt_system.h, and tests. */ #if defined _WIN32 || defined __CYGWIN__ || defined _WIN32_WCE /* DATA imports from DLLs on WIN32 can't be const, because runtime relocations are performed -- see ld's documentation on pseudo-relocs. */ # define LT_DLSYM_CONST #elif defined __osf__ /* This system does not cope well with relocations in const data. */ # define LT_DLSYM_CONST #else # define LT_DLSYM_CONST const #endif #define STREQ(s1, s2) (strcmp ((s1), (s2)) == 0) /* External symbol declarations for the compiler. */\ " if test yes = "$dlself"; then func_verbose "generating symbol list for '$output'" $opt_dry_run || echo ': @PROGRAM@ ' > "$nlist" # Add our own program objects to the symbol list. progfiles=`$ECHO "$objs$old_deplibs" | $SP2NL | $SED "$lo2o" | $NL2SP` for progfile in $progfiles; do func_to_tool_file "$progfile" func_convert_file_msys_to_w32 func_verbose "extracting global C symbols from '$func_to_tool_file_result'" $opt_dry_run || eval "$NM $func_to_tool_file_result | $global_symbol_pipe >> '$nlist'" done if test -n "$exclude_expsyms"; then $opt_dry_run || { eval '$EGREP -v " ($exclude_expsyms)$" "$nlist" > "$nlist"T' eval '$MV "$nlist"T "$nlist"' } fi if test -n "$export_symbols_regex"; then $opt_dry_run || { eval '$EGREP -e "$export_symbols_regex" "$nlist" > "$nlist"T' eval '$MV "$nlist"T "$nlist"' } fi # Prepare the list of exported symbols if test -z "$export_symbols"; then export_symbols=$output_objdir/$outputname.exp $opt_dry_run || { $RM $export_symbols eval "$SED -n -e '/^: @PROGRAM@ $/d' -e 's/^.* \(.*\)$/\1/p' "'< "$nlist" > "$export_symbols"' case $host in *cygwin* | *mingw* | *cegcc* ) eval "echo EXPORTS "'> "$output_objdir/$outputname.def"' eval 'cat "$export_symbols" >> "$output_objdir/$outputname.def"' ;; esac } else $opt_dry_run || { eval "$SED -e 's/\([].[*^$]\)/\\\\\1/g' -e 's/^/ /' -e 's/$/$/'"' < "$export_symbols" > "$output_objdir/$outputname.exp"' eval '$GREP -f "$output_objdir/$outputname.exp" < "$nlist" > "$nlist"T' eval '$MV "$nlist"T "$nlist"' case $host in *cygwin* | *mingw* | *cegcc* ) eval "echo EXPORTS "'> "$output_objdir/$outputname.def"' eval 'cat "$nlist" >> "$output_objdir/$outputname.def"' ;; esac } fi fi for dlprefile in $dlprefiles; do func_verbose "extracting global C symbols from '$dlprefile'" func_basename "$dlprefile" name=$func_basename_result case $host in *cygwin* | *mingw* | *cegcc* ) # if an import library, we need to obtain dlname if func_win32_import_lib_p "$dlprefile"; then func_tr_sh "$dlprefile" eval "curr_lafile=\$libfile_$func_tr_sh_result" dlprefile_dlbasename= if test -n "$curr_lafile" && func_lalib_p "$curr_lafile"; then # Use subshell, to avoid clobbering current variable values dlprefile_dlname=`source "$curr_lafile" && echo "$dlname"` if test -n "$dlprefile_dlname"; then func_basename "$dlprefile_dlname" dlprefile_dlbasename=$func_basename_result else # no lafile. user explicitly requested -dlpreopen <import library>. $sharedlib_from_linklib_cmd "$dlprefile" dlprefile_dlbasename=$sharedlib_from_linklib_result fi fi $opt_dry_run || { if test -n "$dlprefile_dlbasename"; then eval '$ECHO ": $dlprefile_dlbasename" >> "$nlist"' else func_warning "Could not compute DLL name from $name" eval '$ECHO ": $name " >> "$nlist"' fi func_to_tool_file "$dlprefile" func_convert_file_msys_to_w32 eval "$NM \"$func_to_tool_file_result\" 2>/dev/null | $global_symbol_pipe | $SED -e '/I __imp/d' -e 's/I __nm_/D /;s/_nm__//' >> '$nlist'" } else # not an import lib $opt_dry_run || { eval '$ECHO ": $name " >> "$nlist"' func_to_tool_file "$dlprefile" func_convert_file_msys_to_w32 eval "$NM \"$func_to_tool_file_result\" 2>/dev/null | $global_symbol_pipe >> '$nlist'" } fi ;; *) $opt_dry_run || { eval '$ECHO ": $name " >> "$nlist"' func_to_tool_file "$dlprefile" func_convert_file_msys_to_w32 eval "$NM \"$func_to_tool_file_result\" 2>/dev/null | $global_symbol_pipe >> '$nlist'" } ;; esac done $opt_dry_run || { # Make sure we have at least an empty file. test -f "$nlist" || : > "$nlist" if test -n "$exclude_expsyms"; then $EGREP -v " ($exclude_expsyms)$" "$nlist" > "$nlist"T $MV "$nlist"T "$nlist" fi # Try sorting and uniquifying the output. if $GREP -v "^: " < "$nlist" | if sort -k 3 </dev/null >/dev/null 2>&1; then sort -k 3 else sort +2 fi | uniq > "$nlist"S; then : else $GREP -v "^: " < "$nlist" > "$nlist"S fi if test -f "$nlist"S; then eval "$global_symbol_to_cdecl"' < "$nlist"S >> "$output_objdir/$my_dlsyms"' else echo '/* NONE */' >> "$output_objdir/$my_dlsyms" fi func_show_eval '$RM "${nlist}I"' if test -n "$global_symbol_to_import"; then eval "$global_symbol_to_import"' < "$nlist"S > "$nlist"I' fi echo >> "$output_objdir/$my_dlsyms" "\ /* The mapping between symbol names and symbols. */ typedef struct { const char *name; void *address; } lt_dlsymlist; extern LT_DLSYM_CONST lt_dlsymlist lt_${my_prefix}_LTX_preloaded_symbols[];\ " if test -s "$nlist"I; then echo >> "$output_objdir/$my_dlsyms" "\ static void lt_syminit(void) { LT_DLSYM_CONST lt_dlsymlist *symbol = lt_${my_prefix}_LTX_preloaded_symbols; for (; symbol->name; ++symbol) {" $SED 's/.*/ if (STREQ (symbol->name, \"&\")) symbol->address = (void *) \&&;/' < "$nlist"I >> "$output_objdir/$my_dlsyms" echo >> "$output_objdir/$my_dlsyms" "\ } }" fi echo >> "$output_objdir/$my_dlsyms" "\ LT_DLSYM_CONST lt_dlsymlist lt_${my_prefix}_LTX_preloaded_symbols[] = { {\"$my_originator\", (void *) 0}," if test -s "$nlist"I; then echo >> "$output_objdir/$my_dlsyms" "\ {\"@INIT@\", (void *) <_syminit}," fi case $need_lib_prefix in no) eval "$global_symbol_to_c_name_address" < "$nlist" >> "$output_objdir/$my_dlsyms" ;; *) eval "$global_symbol_to_c_name_address_lib_prefix" < "$nlist" >> "$output_objdir/$my_dlsyms" ;; esac echo >> "$output_objdir/$my_dlsyms" "\ {0, (void *) 0} }; /* This works around a problem in FreeBSD linker */ #ifdef FREEBSD_WORKAROUND static const void *lt_preloaded_setup() { return lt_${my_prefix}_LTX_preloaded_symbols; } #endif #ifdef __cplusplus } #endif\ " } # !$opt_dry_run pic_flag_for_symtable= case "$compile_command " in *" -static "*) ;; *) case $host in # compiling the symbol table file with pic_flag works around # a FreeBSD bug that causes programs to crash when -lm is # linked before any other PIC object. But we must not use # pic_flag when linking with -static. The problem exists in # FreeBSD 2.2.6 and is fixed in FreeBSD 3.1. *-*-freebsd2.*|*-*-freebsd3.0*|*-*-freebsdelf3.0*) pic_flag_for_symtable=" $pic_flag -DFREEBSD_WORKAROUND" ;; *-*-hpux*) pic_flag_for_symtable=" $pic_flag" ;; *) $my_pic_p && pic_flag_for_symtable=" $pic_flag" ;; esac ;; esac symtab_cflags= for arg in $LTCFLAGS; do case $arg in -pie | -fpie | -fPIE) ;; *) func_append symtab_cflags " $arg" ;; esac done # Now compile the dynamic symbol file. func_show_eval '(cd $output_objdir && $LTCC$symtab_cflags -c$no_builtin_flag$pic_flag_for_symtable "$my_dlsyms")' 'exit $?' # Clean up the generated files. func_show_eval '$RM "$output_objdir/$my_dlsyms" "$nlist" "${nlist}S" "${nlist}T" "${nlist}I"' # Transform the symbol file into the correct name. symfileobj=$output_objdir/${my_outputname}S.$objext case $host in *cygwin* | *mingw* | *cegcc* ) if test -f "$output_objdir/$my_outputname.def"; then compile_command=`$ECHO "$compile_command" | $SED "s%@SYMFILE@%$output_objdir/$my_outputname.def $symfileobj%"` finalize_command=`$ECHO "$finalize_command" | $SED "s%@SYMFILE@%$output_objdir/$my_outputname.def $symfileobj%"` else compile_command=`$ECHO "$compile_command" | $SED "s%@SYMFILE@%$symfileobj%"` finalize_command=`$ECHO "$finalize_command" | $SED "s%@SYMFILE@%$symfileobj%"` fi ;; *) compile_command=`$ECHO "$compile_command" | $SED "s%@SYMFILE@%$symfileobj%"` finalize_command=`$ECHO "$finalize_command" | $SED "s%@SYMFILE@%$symfileobj%"` ;; esac ;; *) func_fatal_error "unknown suffix for '$my_dlsyms'" ;; esac else # We keep going just in case the user didn't refer to # lt_preloaded_symbols. The linker will fail if global_symbol_pipe # really was required. # Nullify the symbol file. compile_command=`$ECHO "$compile_command" | $SED "s% @SYMFILE@%%"` finalize_command=`$ECHO "$finalize_command" | $SED "s% @SYMFILE@%%"` fi } # func_cygming_gnu_implib_p ARG # This predicate returns with zero status (TRUE) if # ARG is a GNU/binutils-style import library. Returns # with nonzero status (FALSE) otherwise. func_cygming_gnu_implib_p () { $debug_cmd func_to_tool_file "$1" func_convert_file_msys_to_w32 func_cygming_gnu_implib_tmp=`$NM "$func_to_tool_file_result" | eval "$global_symbol_pipe" | $EGREP ' (_head_[A-Za-z0-9_]+_[ad]l*|[A-Za-z0-9_]+_[ad]l*_iname)$'` test -n "$func_cygming_gnu_implib_tmp" } # func_cygming_ms_implib_p ARG # This predicate returns with zero status (TRUE) if # ARG is an MS-style import library. Returns # with nonzero status (FALSE) otherwise. func_cygming_ms_implib_p () { $debug_cmd func_to_tool_file "$1" func_convert_file_msys_to_w32 func_cygming_ms_implib_tmp=`$NM "$func_to_tool_file_result" | eval "$global_symbol_pipe" | $GREP '_NULL_IMPORT_DESCRIPTOR'` test -n "$func_cygming_ms_implib_tmp" } # func_win32_libid arg # return the library type of file 'arg' # # Need a lot of goo to handle *both* DLLs and import libs # Has to be a shell function in order to 'eat' the argument # that is supplied when $file_magic_command is called. # Despite the name, also deal with 64 bit binaries. func_win32_libid () { $debug_cmd win32_libid_type=unknown win32_fileres=`file -L $1 2>/dev/null` case $win32_fileres in *ar\ archive\ import\ library*) # definitely import win32_libid_type="x86 archive import" ;; *ar\ archive*) # could be an import, or static # Keep the egrep pattern in sync with the one in _LT_CHECK_MAGIC_METHOD. if eval $OBJDUMP -f $1 | $SED -e '10q' 2>/dev/null | $EGREP 'file format (pei*-i386(.*architecture: i386)?|pe-arm-wince|pe-x86-64)' >/dev/null; then case $nm_interface in "MS dumpbin") if func_cygming_ms_implib_p "$1" || func_cygming_gnu_implib_p "$1" then win32_nmres=import else win32_nmres= fi ;; *) func_to_tool_file "$1" func_convert_file_msys_to_w32 win32_nmres=`eval $NM -f posix -A \"$func_to_tool_file_result\" | $SED -n -e ' 1,100{ / I /{ s|.*|import| p q } }'` ;; esac case $win32_nmres in import*) win32_libid_type="x86 archive import";; *) win32_libid_type="x86 archive static";; esac fi ;; *DLL*) win32_libid_type="x86 DLL" ;; *executable*) # but shell scripts are "executable" too... case $win32_fileres in *MS\ Windows\ PE\ Intel*) win32_libid_type="x86 DLL" ;; esac ;; esac $ECHO "$win32_libid_type" } # func_cygming_dll_for_implib ARG # # Platform-specific function to extract the # name of the DLL associated with the specified # import library ARG. # Invoked by eval'ing the libtool variable # $sharedlib_from_linklib_cmd # Result is available in the variable # $sharedlib_from_linklib_result func_cygming_dll_for_implib () { $debug_cmd sharedlib_from_linklib_result=`$DLLTOOL --identify-strict --identify "$1"` } # func_cygming_dll_for_implib_fallback_core SECTION_NAME LIBNAMEs # # The is the core of a fallback implementation of a # platform-specific function to extract the name of the # DLL associated with the specified import library LIBNAME. # # SECTION_NAME is either .idata$6 or .idata$7, depending # on the platform and compiler that created the implib. # # Echos the name of the DLL associated with the # specified import library. func_cygming_dll_for_implib_fallback_core () { $debug_cmd match_literal=`$ECHO "$1" | $SED "$sed_make_literal_regex"` $OBJDUMP -s --section "$1" "$2" 2>/dev/null | $SED '/^Contents of section '"$match_literal"':/{ # Place marker at beginning of archive member dllname section s/.*/====MARK====/ p d } # These lines can sometimes be longer than 43 characters, but # are always uninteresting /:[ ]*file format pe[i]\{,1\}-/d /^In archive [^:]*:/d # Ensure marker is printed /^====MARK====/p # Remove all lines with less than 43 characters /^.\{43\}/!d # From remaining lines, remove first 43 characters s/^.\{43\}//' | $SED -n ' # Join marker and all lines until next marker into a single line /^====MARK====/ b para H $ b para b :para x s/\n//g # Remove the marker s/^====MARK====// # Remove trailing dots and whitespace s/[\. \t]*$// # Print /./p' | # we now have a list, one entry per line, of the stringified # contents of the appropriate section of all members of the # archive that possess that section. Heuristic: eliminate # all those that have a first or second character that is # a '.' (that is, objdump's representation of an unprintable # character.) This should work for all archives with less than # 0x302f exports -- but will fail for DLLs whose name actually # begins with a literal '.' or a single character followed by # a '.'. # # Of those that remain, print the first one. $SED -e '/^\./d;/^.\./d;q' } # func_cygming_dll_for_implib_fallback ARG # Platform-specific function to extract the # name of the DLL associated with the specified # import library ARG. # # This fallback implementation is for use when $DLLTOOL # does not support the --identify-strict option. # Invoked by eval'ing the libtool variable # $sharedlib_from_linklib_cmd # Result is available in the variable # $sharedlib_from_linklib_result func_cygming_dll_for_implib_fallback () { $debug_cmd if func_cygming_gnu_implib_p "$1"; then # binutils import library sharedlib_from_linklib_result=`func_cygming_dll_for_implib_fallback_core '.idata$7' "$1"` elif func_cygming_ms_implib_p "$1"; then # ms-generated import library sharedlib_from_linklib_result=`func_cygming_dll_for_implib_fallback_core '.idata$6' "$1"` else # unknown sharedlib_from_linklib_result= fi } # func_extract_an_archive dir oldlib func_extract_an_archive () { $debug_cmd f_ex_an_ar_dir=$1; shift f_ex_an_ar_oldlib=$1 if test yes = "$lock_old_archive_extraction"; then lockfile=$f_ex_an_ar_oldlib.lock until $opt_dry_run || ln "$progpath" "$lockfile" 2>/dev/null; do func_echo "Waiting for $lockfile to be removed" sleep 2 done fi func_show_eval "(cd \$f_ex_an_ar_dir && $AR x \"\$f_ex_an_ar_oldlib\")" \ 'stat=$?; rm -f "$lockfile"; exit $stat' if test yes = "$lock_old_archive_extraction"; then $opt_dry_run || rm -f "$lockfile" fi if ($AR t "$f_ex_an_ar_oldlib" | sort | sort -uc >/dev/null 2>&1); then : else func_fatal_error "object name conflicts in archive: $f_ex_an_ar_dir/$f_ex_an_ar_oldlib" fi } # func_extract_archives gentop oldlib ... func_extract_archives () { $debug_cmd my_gentop=$1; shift my_oldlibs=${1+"$@"} my_oldobjs= my_xlib= my_xabs= my_xdir= for my_xlib in $my_oldlibs; do # Extract the objects. case $my_xlib in [\\/]* | [A-Za-z]:[\\/]*) my_xabs=$my_xlib ;; *) my_xabs=`pwd`"/$my_xlib" ;; esac func_basename "$my_xlib" my_xlib=$func_basename_result my_xlib_u=$my_xlib while :; do case " $extracted_archives " in *" $my_xlib_u "*) func_arith $extracted_serial + 1 extracted_serial=$func_arith_result my_xlib_u=lt$extracted_serial-$my_xlib ;; *) break ;; esac done extracted_archives="$extracted_archives $my_xlib_u" my_xdir=$my_gentop/$my_xlib_u func_mkdir_p "$my_xdir" case $host in *-darwin*) func_verbose "Extracting $my_xabs" # Do not bother doing anything if just a dry run $opt_dry_run || { darwin_orig_dir=`pwd` cd $my_xdir || exit $? darwin_archive=$my_xabs darwin_curdir=`pwd` func_basename "$darwin_archive" darwin_base_archive=$func_basename_result darwin_arches=`$LIPO -info "$darwin_archive" 2>/dev/null | $GREP Architectures 2>/dev/null || true` if test -n "$darwin_arches"; then darwin_arches=`$ECHO "$darwin_arches" | $SED -e 's/.*are://'` darwin_arch= func_verbose "$darwin_base_archive has multiple architectures $darwin_arches" for darwin_arch in $darwin_arches; do func_mkdir_p "unfat-$$/$darwin_base_archive-$darwin_arch" $LIPO -thin $darwin_arch -output "unfat-$$/$darwin_base_archive-$darwin_arch/$darwin_base_archive" "$darwin_archive" cd "unfat-$$/$darwin_base_archive-$darwin_arch" func_extract_an_archive "`pwd`" "$darwin_base_archive" cd "$darwin_curdir" $RM "unfat-$$/$darwin_base_archive-$darwin_arch/$darwin_base_archive" done # $darwin_arches ## Okay now we've a bunch of thin objects, gotta fatten them up :) darwin_filelist=`find unfat-$$ -type f -name \*.o -print -o -name \*.lo -print | $SED -e "$sed_basename" | sort -u` darwin_file= darwin_files= for darwin_file in $darwin_filelist; do darwin_files=`find unfat-$$ -name $darwin_file -print | sort | $NL2SP` $LIPO -create -output "$darwin_file" $darwin_files done # $darwin_filelist $RM -rf unfat-$$ cd "$darwin_orig_dir" else cd $darwin_orig_dir func_extract_an_archive "$my_xdir" "$my_xabs" fi # $darwin_arches } # !$opt_dry_run ;; *) func_extract_an_archive "$my_xdir" "$my_xabs" ;; esac my_oldobjs="$my_oldobjs "`find $my_xdir -name \*.$objext -print -o -name \*.lo -print | sort | $NL2SP` done func_extract_archives_result=$my_oldobjs } # func_emit_wrapper [arg=no] # # Emit a libtool wrapper script on stdout. # Don't directly open a file because we may want to # incorporate the script contents within a cygwin/mingw # wrapper executable. Must ONLY be called from within # func_mode_link because it depends on a number of variables # set therein. # # ARG is the value that the WRAPPER_SCRIPT_BELONGS_IN_OBJDIR # variable will take. If 'yes', then the emitted script # will assume that the directory where it is stored is # the $objdir directory. This is a cygwin/mingw-specific # behavior. func_emit_wrapper () { func_emit_wrapper_arg1=${1-no} $ECHO "\ #! $SHELL # $output - temporary wrapper script for $objdir/$outputname # Generated by $PROGRAM (GNU $PACKAGE) $VERSION # # The $output program cannot be directly executed until all the libtool # libraries that it depends on are installed. # # This wrapper script should never be moved out of the build directory. # If it is, it will not operate correctly. # Sed substitution that helps us do robust quoting. It backslashifies # metacharacters that are still active within double-quoted strings. sed_quote_subst='$sed_quote_subst' # Be Bourne compatible if test -n \"\${ZSH_VERSION+set}\" && (emulate sh) >/dev/null 2>&1; then emulate sh NULLCMD=: # Zsh 3.x and 4.x performs word splitting on \${1+\"\$@\"}, which # is contrary to our usage. Disable this feature. alias -g '\${1+\"\$@\"}'='\"\$@\"' setopt NO_GLOB_SUBST else case \`(set -o) 2>/dev/null\` in *posix*) set -o posix;; esac fi BIN_SH=xpg4; export BIN_SH # for Tru64 DUALCASE=1; export DUALCASE # for MKS sh # The HP-UX ksh and POSIX shell print the target directory to stdout # if CDPATH is set. (unset CDPATH) >/dev/null 2>&1 && unset CDPATH relink_command=\"$relink_command\" # This environment variable determines our operation mode. if test \"\$libtool_install_magic\" = \"$magic\"; then # install mode needs the following variables: generated_by_libtool_version='$macro_version' notinst_deplibs='$notinst_deplibs' else # When we are sourced in execute mode, \$file and \$ECHO are already set. if test \"\$libtool_execute_magic\" != \"$magic\"; then file=\"\$0\"" func_quote_arg pretty "$ECHO" qECHO=$func_quote_arg_result $ECHO "\ # A function that is used when there is no print builtin or printf. func_fallback_echo () { eval 'cat <<_LTECHO_EOF \$1 _LTECHO_EOF' } ECHO=$qECHO fi # Very basic option parsing. These options are (a) specific to # the libtool wrapper, (b) are identical between the wrapper # /script/ and the wrapper /executable/ that is used only on # windows platforms, and (c) all begin with the string "--lt-" # (application programs are unlikely to have options that match # this pattern). # # There are only two supported options: --lt-debug and # --lt-dump-script. There is, deliberately, no --lt-help. # # The first argument to this parsing function should be the # script's $0 value, followed by "$@". lt_option_debug= func_parse_lt_options () { lt_script_arg0=\$0 shift for lt_opt do case \"\$lt_opt\" in --lt-debug) lt_option_debug=1 ;; --lt-dump-script) lt_dump_D=\`\$ECHO \"X\$lt_script_arg0\" | $SED -e 's/^X//' -e 's%/[^/]*$%%'\` test \"X\$lt_dump_D\" = \"X\$lt_script_arg0\" && lt_dump_D=. lt_dump_F=\`\$ECHO \"X\$lt_script_arg0\" | $SED -e 's/^X//' -e 's%^.*/%%'\` cat \"\$lt_dump_D/\$lt_dump_F\" exit 0 ;; --lt-*) \$ECHO \"Unrecognized --lt- option: '\$lt_opt'\" 1>&2 exit 1 ;; esac done # Print the debug banner immediately: if test -n \"\$lt_option_debug\"; then echo \"$outputname:$output:\$LINENO: libtool wrapper (GNU $PACKAGE) $VERSION\" 1>&2 fi } # Used when --lt-debug. Prints its arguments to stdout # (redirection is the responsibility of the caller) func_lt_dump_args () { lt_dump_args_N=1; for lt_arg do \$ECHO \"$outputname:$output:\$LINENO: newargv[\$lt_dump_args_N]: \$lt_arg\" lt_dump_args_N=\`expr \$lt_dump_args_N + 1\` done } # Core function for launching the target application func_exec_program_core () { " case $host in # Backslashes separate directories on plain windows *-*-mingw | *-*-os2* | *-cegcc*) $ECHO "\ if test -n \"\$lt_option_debug\"; then \$ECHO \"$outputname:$output:\$LINENO: newargv[0]: \$progdir\\\\\$program\" 1>&2 func_lt_dump_args \${1+\"\$@\"} 1>&2 fi exec \"\$progdir\\\\\$program\" \${1+\"\$@\"} " ;; *) $ECHO "\ if test -n \"\$lt_option_debug\"; then \$ECHO \"$outputname:$output:\$LINENO: newargv[0]: \$progdir/\$program\" 1>&2 func_lt_dump_args \${1+\"\$@\"} 1>&2 fi exec \"\$progdir/\$program\" \${1+\"\$@\"} " ;; esac $ECHO "\ \$ECHO \"\$0: cannot exec \$program \$*\" 1>&2 exit 1 } # A function to encapsulate launching the target application # Strips options in the --lt-* namespace from \$@ and # launches target application with the remaining arguments. func_exec_program () { case \" \$* \" in *\\ --lt-*) for lt_wr_arg do case \$lt_wr_arg in --lt-*) ;; *) set x \"\$@\" \"\$lt_wr_arg\"; shift;; esac shift done ;; esac func_exec_program_core \${1+\"\$@\"} } # Parse options func_parse_lt_options \"\$0\" \${1+\"\$@\"} # Find the directory that this script lives in. thisdir=\`\$ECHO \"\$file\" | $SED 's%/[^/]*$%%'\` test \"x\$thisdir\" = \"x\$file\" && thisdir=. # Follow symbolic links until we get to the real thisdir. file=\`ls -ld \"\$file\" | $SED -n 's/.*-> //p'\` while test -n \"\$file\"; do destdir=\`\$ECHO \"\$file\" | $SED 's%/[^/]*\$%%'\` # If there was a directory component, then change thisdir. if test \"x\$destdir\" != \"x\$file\"; then case \"\$destdir\" in [\\\\/]* | [A-Za-z]:[\\\\/]*) thisdir=\"\$destdir\" ;; *) thisdir=\"\$thisdir/\$destdir\" ;; esac fi file=\`\$ECHO \"\$file\" | $SED 's%^.*/%%'\` file=\`ls -ld \"\$thisdir/\$file\" | $SED -n 's/.*-> //p'\` done # Usually 'no', except on cygwin/mingw when embedded into # the cwrapper. WRAPPER_SCRIPT_BELONGS_IN_OBJDIR=$func_emit_wrapper_arg1 if test \"\$WRAPPER_SCRIPT_BELONGS_IN_OBJDIR\" = \"yes\"; then # special case for '.' if test \"\$thisdir\" = \".\"; then thisdir=\`pwd\` fi # remove .libs from thisdir case \"\$thisdir\" in *[\\\\/]$objdir ) thisdir=\`\$ECHO \"\$thisdir\" | $SED 's%[\\\\/][^\\\\/]*$%%'\` ;; $objdir ) thisdir=. ;; esac fi # Try to get the absolute directory name. absdir=\`cd \"\$thisdir\" && pwd\` test -n \"\$absdir\" && thisdir=\"\$absdir\" " if test yes = "$fast_install"; then $ECHO "\ program=lt-'$outputname'$exeext progdir=\"\$thisdir/$objdir\" if test ! -f \"\$progdir/\$program\" || { file=\`ls -1dt \"\$progdir/\$program\" \"\$progdir/../\$program\" 2>/dev/null | $SED 1q\`; \\ test \"X\$file\" != \"X\$progdir/\$program\"; }; then file=\"\$\$-\$program\" if test ! -d \"\$progdir\"; then $MKDIR \"\$progdir\" else $RM \"\$progdir/\$file\" fi" $ECHO "\ # relink executable if necessary if test -n \"\$relink_command\"; then if relink_command_output=\`eval \$relink_command 2>&1\`; then : else \$ECHO \"\$relink_command_output\" >&2 $RM \"\$progdir/\$file\" exit 1 fi fi $MV \"\$progdir/\$file\" \"\$progdir/\$program\" 2>/dev/null || { $RM \"\$progdir/\$program\"; $MV \"\$progdir/\$file\" \"\$progdir/\$program\"; } $RM \"\$progdir/\$file\" fi" else $ECHO "\ program='$outputname' progdir=\"\$thisdir/$objdir\" " fi $ECHO "\ if test -f \"\$progdir/\$program\"; then" # fixup the dll searchpath if we need to. # # Fix the DLL searchpath if we need to. Do this before prepending # to shlibpath, because on Windows, both are PATH and uninstalled # libraries must come first. if test -n "$dllsearchpath"; then $ECHO "\ # Add the dll search path components to the executable PATH PATH=$dllsearchpath:\$PATH " fi # Export our shlibpath_var if we have one. if test yes = "$shlibpath_overrides_runpath" && test -n "$shlibpath_var" && test -n "$temp_rpath"; then $ECHO "\ # Add our own library path to $shlibpath_var $shlibpath_var=\"$temp_rpath\$$shlibpath_var\" # Some systems cannot cope with colon-terminated $shlibpath_var # The second colon is a workaround for a bug in BeOS R4 sed $shlibpath_var=\`\$ECHO \"\$$shlibpath_var\" | $SED 's/::*\$//'\` export $shlibpath_var " fi $ECHO "\ if test \"\$libtool_execute_magic\" != \"$magic\"; then # Run the actual program with our arguments. func_exec_program \${1+\"\$@\"} fi else # The program doesn't exist. \$ECHO \"\$0: error: '\$progdir/\$program' does not exist\" 1>&2 \$ECHO \"This script is just a wrapper for \$program.\" 1>&2 \$ECHO \"See the $PACKAGE documentation for more information.\" 1>&2 exit 1 fi fi\ " } # func_emit_cwrapperexe_src # emit the source code for a wrapper executable on stdout # Must ONLY be called from within func_mode_link because # it depends on a number of variable set therein. func_emit_cwrapperexe_src () { cat <<EOF /* $cwrappersource - temporary wrapper executable for $objdir/$outputname Generated by $PROGRAM (GNU $PACKAGE) $VERSION The $output program cannot be directly executed until all the libtool libraries that it depends on are installed. This wrapper executable should never be moved out of the build directory. If it is, it will not operate correctly. */ EOF cat <<"EOF" #ifdef _MSC_VER # define _CRT_SECURE_NO_DEPRECATE 1 #endif #include <stdio.h> #include <stdlib.h> #ifdef _MSC_VER # include <direct.h> # include <process.h> # include <io.h> #else # include <unistd.h> # include <stdint.h> # ifdef __CYGWIN__ # include <io.h> # endif #endif #include <malloc.h> #include <stdarg.h> #include <assert.h> #include <string.h> #include <ctype.h> #include <errno.h> #include <fcntl.h> #include <sys/stat.h> #define STREQ(s1, s2) (strcmp ((s1), (s2)) == 0) /* declarations of non-ANSI functions */ #if defined __MINGW32__ # ifdef __STRICT_ANSI__ int _putenv (const char *); # endif #elif defined __CYGWIN__ # ifdef __STRICT_ANSI__ char *realpath (const char *, char *); int putenv (char *); int setenv (const char *, const char *, int); # endif /* #elif defined other_platform || defined ... */ #endif /* portability defines, excluding path handling macros */ #if defined _MSC_VER # define setmode _setmode # define stat _stat # define chmod _chmod # define getcwd _getcwd # define putenv _putenv # define S_IXUSR _S_IEXEC #elif defined __MINGW32__ # define setmode _setmode # define stat _stat # define chmod _chmod # define getcwd _getcwd # define putenv _putenv #elif defined __CYGWIN__ # define HAVE_SETENV # define FOPEN_WB "wb" /* #elif defined other platforms ... */ #endif #if defined PATH_MAX # define LT_PATHMAX PATH_MAX #elif defined MAXPATHLEN # define LT_PATHMAX MAXPATHLEN #else # define LT_PATHMAX 1024 #endif #ifndef S_IXOTH # define S_IXOTH 0 #endif #ifndef S_IXGRP # define S_IXGRP 0 #endif /* path handling portability macros */ #ifndef DIR_SEPARATOR # define DIR_SEPARATOR '/' # define PATH_SEPARATOR ':' #endif #if defined _WIN32 || defined __MSDOS__ || defined __DJGPP__ || \ defined __OS2__ # define HAVE_DOS_BASED_FILE_SYSTEM # define FOPEN_WB "wb" # ifndef DIR_SEPARATOR_2 # define DIR_SEPARATOR_2 '\\' # endif # ifndef PATH_SEPARATOR_2 # define PATH_SEPARATOR_2 ';' # endif #endif #ifndef DIR_SEPARATOR_2 # define IS_DIR_SEPARATOR(ch) ((ch) == DIR_SEPARATOR) #else /* DIR_SEPARATOR_2 */ # define IS_DIR_SEPARATOR(ch) \ (((ch) == DIR_SEPARATOR) || ((ch) == DIR_SEPARATOR_2)) #endif /* DIR_SEPARATOR_2 */ #ifndef PATH_SEPARATOR_2 # define IS_PATH_SEPARATOR(ch) ((ch) == PATH_SEPARATOR) #else /* PATH_SEPARATOR_2 */ # define IS_PATH_SEPARATOR(ch) ((ch) == PATH_SEPARATOR_2) #endif /* PATH_SEPARATOR_2 */ #ifndef FOPEN_WB # define FOPEN_WB "w" #endif #ifndef _O_BINARY # define _O_BINARY 0 #endif #define XMALLOC(type, num) ((type *) xmalloc ((num) * sizeof(type))) #define XFREE(stale) do { \ if (stale) { free (stale); stale = 0; } \ } while (0) #if defined LT_DEBUGWRAPPER static int lt_debug = 1; #else static int lt_debug = 0; #endif const char *program_name = "libtool-wrapper"; /* in case xstrdup fails */ void *xmalloc (size_t num); char *xstrdup (const char *string); const char *base_name (const char *name); char *find_executable (const char *wrapper); char *chase_symlinks (const char *pathspec); int make_executable (const char *path); int check_executable (const char *path); char *strendzap (char *str, const char *pat); void lt_debugprintf (const char *file, int line, const char *fmt, ...); void lt_fatal (const char *file, int line, const char *message, ...); static const char *nonnull (const char *s); static const char *nonempty (const char *s); void lt_setenv (const char *name, const char *value); char *lt_extend_str (const char *orig_value, const char *add, int to_end); void lt_update_exe_path (const char *name, const char *value); void lt_update_lib_path (const char *name, const char *value); char **prepare_spawn (char **argv); void lt_dump_script (FILE *f); EOF cat <<EOF #if __GNUC__ < 4 || (__GNUC__ == 4 && __GNUC_MINOR__ < 5) # define externally_visible volatile #else # define externally_visible __attribute__((externally_visible)) volatile #endif externally_visible const char * MAGIC_EXE = "$magic_exe"; const char * LIB_PATH_VARNAME = "$shlibpath_var"; EOF if test yes = "$shlibpath_overrides_runpath" && test -n "$shlibpath_var" && test -n "$temp_rpath"; then func_to_host_path "$temp_rpath" cat <<EOF const char * LIB_PATH_VALUE = "$func_to_host_path_result"; EOF else cat <<"EOF" const char * LIB_PATH_VALUE = ""; EOF fi if test -n "$dllsearchpath"; then func_to_host_path "$dllsearchpath:" cat <<EOF const char * EXE_PATH_VARNAME = "PATH"; const char * EXE_PATH_VALUE = "$func_to_host_path_result"; EOF else cat <<"EOF" const char * EXE_PATH_VARNAME = ""; const char * EXE_PATH_VALUE = ""; EOF fi if test yes = "$fast_install"; then cat <<EOF const char * TARGET_PROGRAM_NAME = "lt-$outputname"; /* hopefully, no .exe */ EOF else cat <<EOF const char * TARGET_PROGRAM_NAME = "$outputname"; /* hopefully, no .exe */ EOF fi cat <<"EOF" #define LTWRAPPER_OPTION_PREFIX "--lt-" static const char *ltwrapper_option_prefix = LTWRAPPER_OPTION_PREFIX; static const char *dumpscript_opt = LTWRAPPER_OPTION_PREFIX "dump-script"; static const char *debug_opt = LTWRAPPER_OPTION_PREFIX "debug"; int main (int argc, char *argv[]) { char **newargz; int newargc; char *tmp_pathspec; char *actual_cwrapper_path; char *actual_cwrapper_name; char *target_name; char *lt_argv_zero; int rval = 127; int i; program_name = (char *) xstrdup (base_name (argv[0])); newargz = XMALLOC (char *, (size_t) argc + 1); /* very simple arg parsing; don't want to rely on getopt * also, copy all non cwrapper options to newargz, except * argz[0], which is handled differently */ newargc=0; for (i = 1; i < argc; i++) { if (STREQ (argv[i], dumpscript_opt)) { EOF case $host in *mingw* | *cygwin* ) # make stdout use "unix" line endings echo " setmode(1,_O_BINARY);" ;; esac cat <<"EOF" lt_dump_script (stdout); return 0; } if (STREQ (argv[i], debug_opt)) { lt_debug = 1; continue; } if (STREQ (argv[i], ltwrapper_option_prefix)) { /* however, if there is an option in the LTWRAPPER_OPTION_PREFIX namespace, but it is not one of the ones we know about and have already dealt with, above (inluding dump-script), then report an error. Otherwise, targets might begin to believe they are allowed to use options in the LTWRAPPER_OPTION_PREFIX namespace. The first time any user complains about this, we'll need to make LTWRAPPER_OPTION_PREFIX a configure-time option or a configure.ac-settable value. */ lt_fatal (__FILE__, __LINE__, "unrecognized %s option: '%s'", ltwrapper_option_prefix, argv[i]); } /* otherwise ... */ newargz[++newargc] = xstrdup (argv[i]); } newargz[++newargc] = NULL; EOF cat <<EOF /* The GNU banner must be the first non-error debug message */ lt_debugprintf (__FILE__, __LINE__, "libtool wrapper (GNU $PACKAGE) $VERSION\n"); EOF cat <<"EOF" lt_debugprintf (__FILE__, __LINE__, "(main) argv[0]: %s\n", argv[0]); lt_debugprintf (__FILE__, __LINE__, "(main) program_name: %s\n", program_name); tmp_pathspec = find_executable (argv[0]); if (tmp_pathspec == NULL) lt_fatal (__FILE__, __LINE__, "couldn't find %s", argv[0]); lt_debugprintf (__FILE__, __LINE__, "(main) found exe (before symlink chase) at: %s\n", tmp_pathspec); actual_cwrapper_path = chase_symlinks (tmp_pathspec); lt_debugprintf (__FILE__, __LINE__, "(main) found exe (after symlink chase) at: %s\n", actual_cwrapper_path); XFREE (tmp_pathspec); actual_cwrapper_name = xstrdup (base_name (actual_cwrapper_path)); strendzap (actual_cwrapper_path, actual_cwrapper_name); /* wrapper name transforms */ strendzap (actual_cwrapper_name, ".exe"); tmp_pathspec = lt_extend_str (actual_cwrapper_name, ".exe", 1); XFREE (actual_cwrapper_name); actual_cwrapper_name = tmp_pathspec; tmp_pathspec = 0; /* target_name transforms -- use actual target program name; might have lt- prefix */ target_name = xstrdup (base_name (TARGET_PROGRAM_NAME)); strendzap (target_name, ".exe"); tmp_pathspec = lt_extend_str (target_name, ".exe", 1); XFREE (target_name); target_name = tmp_pathspec; tmp_pathspec = 0; lt_debugprintf (__FILE__, __LINE__, "(main) libtool target name: %s\n", target_name); EOF cat <<EOF newargz[0] = XMALLOC (char, (strlen (actual_cwrapper_path) + strlen ("$objdir") + 1 + strlen (actual_cwrapper_name) + 1)); strcpy (newargz[0], actual_cwrapper_path); strcat (newargz[0], "$objdir"); strcat (newargz[0], "/"); EOF cat <<"EOF" /* stop here, and copy so we don't have to do this twice */ tmp_pathspec = xstrdup (newargz[0]); /* do NOT want the lt- prefix here, so use actual_cwrapper_name */ strcat (newargz[0], actual_cwrapper_name); /* DO want the lt- prefix here if it exists, so use target_name */ lt_argv_zero = lt_extend_str (tmp_pathspec, target_name, 1); XFREE (tmp_pathspec); tmp_pathspec = NULL; EOF case $host_os in mingw*) cat <<"EOF" { char* p; while ((p = strchr (newargz[0], '\\')) != NULL) { *p = '/'; } while ((p = strchr (lt_argv_zero, '\\')) != NULL) { *p = '/'; } } EOF ;; esac cat <<"EOF" XFREE (target_name); XFREE (actual_cwrapper_path); XFREE (actual_cwrapper_name); lt_setenv ("BIN_SH", "xpg4"); /* for Tru64 */ lt_setenv ("DUALCASE", "1"); /* for MSK sh */ /* Update the DLL searchpath. EXE_PATH_VALUE ($dllsearchpath) must be prepended before (that is, appear after) LIB_PATH_VALUE ($temp_rpath) because on Windows, both *_VARNAMEs are PATH but uninstalled libraries must come first. */ lt_update_exe_path (EXE_PATH_VARNAME, EXE_PATH_VALUE); lt_update_lib_path (LIB_PATH_VARNAME, LIB_PATH_VALUE); lt_debugprintf (__FILE__, __LINE__, "(main) lt_argv_zero: %s\n", nonnull (lt_argv_zero)); for (i = 0; i < newargc; i++) { lt_debugprintf (__FILE__, __LINE__, "(main) newargz[%d]: %s\n", i, nonnull (newargz[i])); } EOF case $host_os in mingw*) cat <<"EOF" /* execv doesn't actually work on mingw as expected on unix */ newargz = prepare_spawn (newargz); rval = (int) _spawnv (_P_WAIT, lt_argv_zero, (const char * const *) newargz); if (rval == -1) { /* failed to start process */ lt_debugprintf (__FILE__, __LINE__, "(main) failed to launch target \"%s\": %s\n", lt_argv_zero, nonnull (strerror (errno))); return 127; } return rval; EOF ;; *) cat <<"EOF" execv (lt_argv_zero, newargz); return rval; /* =127, but avoids unused variable warning */ EOF ;; esac cat <<"EOF" } void * xmalloc (size_t num) { void *p = (void *) malloc (num); if (!p) lt_fatal (__FILE__, __LINE__, "memory exhausted"); return p; } char * xstrdup (const char *string) { return string ? strcpy ((char *) xmalloc (strlen (string) + 1), string) : NULL; } const char * base_name (const char *name) { const char *base; #if defined HAVE_DOS_BASED_FILE_SYSTEM /* Skip over the disk name in MSDOS pathnames. */ if (isalpha ((unsigned char) name[0]) && name[1] == ':') name += 2; #endif for (base = name; *name; name++) if (IS_DIR_SEPARATOR (*name)) base = name + 1; return base; } int check_executable (const char *path) { struct stat st; lt_debugprintf (__FILE__, __LINE__, "(check_executable): %s\n", nonempty (path)); if ((!path) || (!*path)) return 0; if ((stat (path, &st) >= 0) && (st.st_mode & (S_IXUSR | S_IXGRP | S_IXOTH))) return 1; else return 0; } int make_executable (const char *path) { int rval = 0; struct stat st; lt_debugprintf (__FILE__, __LINE__, "(make_executable): %s\n", nonempty (path)); if ((!path) || (!*path)) return 0; if (stat (path, &st) >= 0) { rval = chmod (path, st.st_mode | S_IXOTH | S_IXGRP | S_IXUSR); } return rval; } /* Searches for the full path of the wrapper. Returns newly allocated full path name if found, NULL otherwise Does not chase symlinks, even on platforms that support them. */ char * find_executable (const char *wrapper) { int has_slash = 0; const char *p; const char *p_next; /* static buffer for getcwd */ char tmp[LT_PATHMAX + 1]; size_t tmp_len; char *concat_name; lt_debugprintf (__FILE__, __LINE__, "(find_executable): %s\n", nonempty (wrapper)); if ((wrapper == NULL) || (*wrapper == '\0')) return NULL; /* Absolute path? */ #if defined HAVE_DOS_BASED_FILE_SYSTEM if (isalpha ((unsigned char) wrapper[0]) && wrapper[1] == ':') { concat_name = xstrdup (wrapper); if (check_executable (concat_name)) return concat_name; XFREE (concat_name); } else { #endif if (IS_DIR_SEPARATOR (wrapper[0])) { concat_name = xstrdup (wrapper); if (check_executable (concat_name)) return concat_name; XFREE (concat_name); } #if defined HAVE_DOS_BASED_FILE_SYSTEM } #endif for (p = wrapper; *p; p++) if (*p == '/') { has_slash = 1; break; } if (!has_slash) { /* no slashes; search PATH */ const char *path = getenv ("PATH"); if (path != NULL) { for (p = path; *p; p = p_next) { const char *q; size_t p_len; for (q = p; *q; q++) if (IS_PATH_SEPARATOR (*q)) break; p_len = (size_t) (q - p); p_next = (*q == '\0' ? q : q + 1); if (p_len == 0) { /* empty path: current directory */ if (getcwd (tmp, LT_PATHMAX) == NULL) lt_fatal (__FILE__, __LINE__, "getcwd failed: %s", nonnull (strerror (errno))); tmp_len = strlen (tmp); concat_name = XMALLOC (char, tmp_len + 1 + strlen (wrapper) + 1); memcpy (concat_name, tmp, tmp_len); concat_name[tmp_len] = '/'; strcpy (concat_name + tmp_len + 1, wrapper); } else { concat_name = XMALLOC (char, p_len + 1 + strlen (wrapper) + 1); memcpy (concat_name, p, p_len); concat_name[p_len] = '/'; strcpy (concat_name + p_len + 1, wrapper); } if (check_executable (concat_name)) return concat_name; XFREE (concat_name); } } /* not found in PATH; assume curdir */ } /* Relative path | not found in path: prepend cwd */ if (getcwd (tmp, LT_PATHMAX) == NULL) lt_fatal (__FILE__, __LINE__, "getcwd failed: %s", nonnull (strerror (errno))); tmp_len = strlen (tmp); concat_name = XMALLOC (char, tmp_len + 1 + strlen (wrapper) + 1); memcpy (concat_name, tmp, tmp_len); concat_name[tmp_len] = '/'; strcpy (concat_name + tmp_len + 1, wrapper); if (check_executable (concat_name)) return concat_name; XFREE (concat_name); return NULL; } char * chase_symlinks (const char *pathspec) { #ifndef S_ISLNK return xstrdup (pathspec); #else char buf[LT_PATHMAX]; struct stat s; char *tmp_pathspec = xstrdup (pathspec); char *p; int has_symlinks = 0; while (strlen (tmp_pathspec) && !has_symlinks) { lt_debugprintf (__FILE__, __LINE__, "checking path component for symlinks: %s\n", tmp_pathspec); if (lstat (tmp_pathspec, &s) == 0) { if (S_ISLNK (s.st_mode) != 0) { has_symlinks = 1; break; } /* search backwards for last DIR_SEPARATOR */ p = tmp_pathspec + strlen (tmp_pathspec) - 1; while ((p > tmp_pathspec) && (!IS_DIR_SEPARATOR (*p))) p--; if ((p == tmp_pathspec) && (!IS_DIR_SEPARATOR (*p))) { /* no more DIR_SEPARATORS left */ break; } *p = '\0'; } else { lt_fatal (__FILE__, __LINE__, "error accessing file \"%s\": %s", tmp_pathspec, nonnull (strerror (errno))); } } XFREE (tmp_pathspec); if (!has_symlinks) { return xstrdup (pathspec); } tmp_pathspec = realpath (pathspec, buf); if (tmp_pathspec == 0) { lt_fatal (__FILE__, __LINE__, "could not follow symlinks for %s", pathspec); } return xstrdup (tmp_pathspec); #endif } char * strendzap (char *str, const char *pat) { size_t len, patlen; assert (str != NULL); assert (pat != NULL); len = strlen (str); patlen = strlen (pat); if (patlen <= len) { str += len - patlen; if (STREQ (str, pat)) *str = '\0'; } return str; } void lt_debugprintf (const char *file, int line, const char *fmt, ...) { va_list args; if (lt_debug) { (void) fprintf (stderr, "%s:%s:%d: ", program_name, file, line); va_start (args, fmt); (void) vfprintf (stderr, fmt, args); va_end (args); } } static void lt_error_core (int exit_status, const char *file, int line, const char *mode, const char *message, va_list ap) { fprintf (stderr, "%s:%s:%d: %s: ", program_name, file, line, mode); vfprintf (stderr, message, ap); fprintf (stderr, ".\n"); if (exit_status >= 0) exit (exit_status); } void lt_fatal (const char *file, int line, const char *message, ...) { va_list ap; va_start (ap, message); lt_error_core (EXIT_FAILURE, file, line, "FATAL", message, ap); va_end (ap); } static const char * nonnull (const char *s) { return s ? s : "(null)"; } static const char * nonempty (const char *s) { return (s && !*s) ? "(empty)" : nonnull (s); } void lt_setenv (const char *name, const char *value) { lt_debugprintf (__FILE__, __LINE__, "(lt_setenv) setting '%s' to '%s'\n", nonnull (name), nonnull (value)); { #ifdef HAVE_SETENV /* always make a copy, for consistency with !HAVE_SETENV */ char *str = xstrdup (value); setenv (name, str, 1); #else size_t len = strlen (name) + 1 + strlen (value) + 1; char *str = XMALLOC (char, len); sprintf (str, "%s=%s", name, value); if (putenv (str) != EXIT_SUCCESS) { XFREE (str); } #endif } } char * lt_extend_str (const char *orig_value, const char *add, int to_end) { char *new_value; if (orig_value && *orig_value) { size_t orig_value_len = strlen (orig_value); size_t add_len = strlen (add); new_value = XMALLOC (char, add_len + orig_value_len + 1); if (to_end) { strcpy (new_value, orig_value); strcpy (new_value + orig_value_len, add); } else { strcpy (new_value, add); strcpy (new_value + add_len, orig_value); } } else { new_value = xstrdup (add); } return new_value; } void lt_update_exe_path (const char *name, const char *value) { lt_debugprintf (__FILE__, __LINE__, "(lt_update_exe_path) modifying '%s' by prepending '%s'\n", nonnull (name), nonnull (value)); if (name && *name && value && *value) { char *new_value = lt_extend_str (getenv (name), value, 0); /* some systems can't cope with a ':'-terminated path #' */ size_t len = strlen (new_value); while ((len > 0) && IS_PATH_SEPARATOR (new_value[len-1])) { new_value[--len] = '\0'; } lt_setenv (name, new_value); XFREE (new_value); } } void lt_update_lib_path (const char *name, const char *value) { lt_debugprintf (__FILE__, __LINE__, "(lt_update_lib_path) modifying '%s' by prepending '%s'\n", nonnull (name), nonnull (value)); if (name && *name && value && *value) { char *new_value = lt_extend_str (getenv (name), value, 0); lt_setenv (name, new_value); XFREE (new_value); } } EOF case $host_os in mingw*) cat <<"EOF" /* Prepares an argument vector before calling spawn(). Note that spawn() does not by itself call the command interpreter (getenv ("COMSPEC") != NULL ? getenv ("COMSPEC") : ({ OSVERSIONINFO v; v.dwOSVersionInfoSize = sizeof(OSVERSIONINFO); GetVersionEx(&v); v.dwPlatformId == VER_PLATFORM_WIN32_NT; }) ? "cmd.exe" : "command.com"). Instead it simply concatenates the arguments, separated by ' ', and calls CreateProcess(). We must quote the arguments since Win32 CreateProcess() interprets characters like ' ', '\t', '\\', '"' (but not '<' and '>') in a special way: - Space and tab are interpreted as delimiters. They are not treated as delimiters if they are surrounded by double quotes: "...". - Unescaped double quotes are removed from the input. Their only effect is that within double quotes, space and tab are treated like normal characters. - Backslashes not followed by double quotes are not special. - But 2*n+1 backslashes followed by a double quote become n backslashes followed by a double quote (n >= 0): \" -> " \\\" -> \" \\\\\" -> \\" */ #define SHELL_SPECIAL_CHARS "\"\\ \001\002\003\004\005\006\007\010\011\012\013\014\015\016\017\020\021\022\023\024\025\026\027\030\031\032\033\034\035\036\037" #define SHELL_SPACE_CHARS " \001\002\003\004\005\006\007\010\011\012\013\014\015\016\017\020\021\022\023\024\025\026\027\030\031\032\033\034\035\036\037" char ** prepare_spawn (char **argv) { size_t argc; char **new_argv; size_t i; /* Count number of arguments. */ for (argc = 0; argv[argc] != NULL; argc++) ; /* Allocate new argument vector. */ new_argv = XMALLOC (char *, argc + 1); /* Put quoted arguments into the new argument vector. */ for (i = 0; i < argc; i++) { const char *string = argv[i]; if (string[0] == '\0') new_argv[i] = xstrdup ("\"\""); else if (strpbrk (string, SHELL_SPECIAL_CHARS) != NULL) { int quote_around = (strpbrk (string, SHELL_SPACE_CHARS) != NULL); size_t length; unsigned int backslashes; const char *s; char *quoted_string; char *p; length = 0; backslashes = 0; if (quote_around) length++; for (s = string; *s != '\0'; s++) { char c = *s; if (c == '"') length += backslashes + 1; length++; if (c == '\\') backslashes++; else backslashes = 0; } if (quote_around) length += backslashes + 1; quoted_string = XMALLOC (char, length + 1); p = quoted_string; backslashes = 0; if (quote_around) *p++ = '"'; for (s = string; *s != '\0'; s++) { char c = *s; if (c == '"') { unsigned int j; for (j = backslashes + 1; j > 0; j--) *p++ = '\\'; } *p++ = c; if (c == '\\') backslashes++; else backslashes = 0; } if (quote_around) { unsigned int j; for (j = backslashes; j > 0; j--) *p++ = '\\'; *p++ = '"'; } *p = '\0'; new_argv[i] = quoted_string; } else new_argv[i] = (char *) string; } new_argv[argc] = NULL; return new_argv; } EOF ;; esac cat <<"EOF" void lt_dump_script (FILE* f) { EOF func_emit_wrapper yes | $SED -n -e ' s/^\(.\{79\}\)\(..*\)/\1\ \2/ h s/\([\\"]\)/\\\1/g s/$/\\n/ s/\([^\n]*\).*/ fputs ("\1", f);/p g D' cat <<"EOF" } EOF } # end: func_emit_cwrapperexe_src # func_win32_import_lib_p ARG # True if ARG is an import lib, as indicated by $file_magic_cmd func_win32_import_lib_p () { $debug_cmd case `eval $file_magic_cmd \"\$1\" 2>/dev/null | $SED -e 10q` in *import*) : ;; *) false ;; esac } # func_suncc_cstd_abi # !!ONLY CALL THIS FOR SUN CC AFTER $compile_command IS FULLY EXPANDED!! # Several compiler flags select an ABI that is incompatible with the # Cstd library. Avoid specifying it if any are in CXXFLAGS. func_suncc_cstd_abi () { $debug_cmd case " $compile_command " in *" -compat=g "*|*\ -std=c++[0-9][0-9]\ *|*" -library=stdcxx4 "*|*" -library=stlport4 "*) suncc_use_cstd_abi=no ;; *) suncc_use_cstd_abi=yes ;; esac } # func_mode_link arg... func_mode_link () { $debug_cmd case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-os2* | *-cegcc*) # It is impossible to link a dll without this setting, and # we shouldn't force the makefile maintainer to figure out # what system we are compiling for in order to pass an extra # flag for every libtool invocation. # allow_undefined=no # FIXME: Unfortunately, there are problems with the above when trying # to make a dll that has undefined symbols, in which case not # even a static library is built. For now, we need to specify # -no-undefined on the libtool link line when we can be certain # that all symbols are satisfied, otherwise we get a static library. allow_undefined=yes ;; *) allow_undefined=yes ;; esac libtool_args=$nonopt base_compile="$nonopt $@" compile_command=$nonopt finalize_command=$nonopt compile_rpath= finalize_rpath= compile_shlibpath= finalize_shlibpath= convenience= old_convenience= deplibs= old_deplibs= compiler_flags= linker_flags= dllsearchpath= lib_search_path=`pwd` inst_prefix_dir= new_inherited_linker_flags= avoid_version=no bindir= dlfiles= dlprefiles= dlself=no export_dynamic=no export_symbols= export_symbols_regex= generated= libobjs= ltlibs= module=no no_install=no objs= os2dllname= non_pic_objects= precious_files_regex= prefer_static_libs=no preload=false prev= prevarg= release= rpath= xrpath= perm_rpath= temp_rpath= thread_safe=no vinfo= vinfo_number=no weak_libs= single_module=$wl-single_module func_infer_tag $base_compile # We need to know -static, to get the right output filenames. for arg do case $arg in -shared) test yes != "$build_libtool_libs" \ && func_fatal_configuration "cannot build a shared library" build_old_libs=no break ;; -all-static | -static | -static-libtool-libs) case $arg in -all-static) if test yes = "$build_libtool_libs" && test -z "$link_static_flag"; then func_warning "complete static linking is impossible in this configuration" fi if test -n "$link_static_flag"; then dlopen_self=$dlopen_self_static fi prefer_static_libs=yes ;; -static) if test -z "$pic_flag" && test -n "$link_static_flag"; then dlopen_self=$dlopen_self_static fi prefer_static_libs=built ;; -static-libtool-libs) if test -z "$pic_flag" && test -n "$link_static_flag"; then dlopen_self=$dlopen_self_static fi prefer_static_libs=yes ;; esac build_libtool_libs=no build_old_libs=yes break ;; esac done # See if our shared archives depend on static archives. test -n "$old_archive_from_new_cmds" && build_old_libs=yes # Go through the arguments, transforming them on the way. while test "$#" -gt 0; do arg=$1 shift func_quote_arg pretty,unquoted "$arg" qarg=$func_quote_arg_unquoted_result func_append libtool_args " $func_quote_arg_result" # If the previous option needs an argument, assign it. if test -n "$prev"; then case $prev in output) func_append compile_command " @OUTPUT@" func_append finalize_command " @OUTPUT@" ;; esac case $prev in bindir) bindir=$arg prev= continue ;; dlfiles|dlprefiles) $preload || { # Add the symbol object into the linking commands. func_append compile_command " @SYMFILE@" func_append finalize_command " @SYMFILE@" preload=: } case $arg in *.la | *.lo) ;; # We handle these cases below. force) if test no = "$dlself"; then dlself=needless export_dynamic=yes fi prev= continue ;; self) if test dlprefiles = "$prev"; then dlself=yes elif test dlfiles = "$prev" && test yes != "$dlopen_self"; then dlself=yes else dlself=needless export_dynamic=yes fi prev= continue ;; *) if test dlfiles = "$prev"; then func_append dlfiles " $arg" else func_append dlprefiles " $arg" fi prev= continue ;; esac ;; expsyms) export_symbols=$arg test -f "$arg" \ || func_fatal_error "symbol file '$arg' does not exist" prev= continue ;; expsyms_regex) export_symbols_regex=$arg prev= continue ;; framework) case $host in *-*-darwin*) case "$deplibs " in *" $qarg.ltframework "*) ;; *) func_append deplibs " $qarg.ltframework" # this is fixed later ;; esac ;; esac prev= continue ;; inst_prefix) inst_prefix_dir=$arg prev= continue ;; mllvm) # Clang does not use LLVM to link, so we can simply discard any # '-mllvm $arg' options when doing the link step. prev= continue ;; objectlist) if test -f "$arg"; then save_arg=$arg moreargs= for fil in `cat "$save_arg"` do # func_append moreargs " $fil" arg=$fil # A libtool-controlled object. # Check to see that this really is a libtool object. if func_lalib_unsafe_p "$arg"; then pic_object= non_pic_object= # Read the .lo file func_source "$arg" if test -z "$pic_object" || test -z "$non_pic_object" || test none = "$pic_object" && test none = "$non_pic_object"; then func_fatal_error "cannot find name of object for '$arg'" fi # Extract subdirectory from the argument. func_dirname "$arg" "/" "" xdir=$func_dirname_result if test none != "$pic_object"; then # Prepend the subdirectory the object is found in. pic_object=$xdir$pic_object if test dlfiles = "$prev"; 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then if test yes = "$build_libtool_libs" && test yes = "$dlopen_support"; then func_append dlfiles " $pic_object" prev= continue else # If libtool objects are unsupported, then we need to preload. prev=dlprefiles fi fi # CHECK ME: I think I busted this. -Ossama if test dlprefiles = "$prev"; then # Preload the old-style object. func_append dlprefiles " $pic_object" prev= fi # A PIC object. func_append libobjs " $pic_object" arg=$pic_object } # Non-PIC object. if test none != "$non_pic_object"; then # Prepend the subdirectory the object is found in. non_pic_object=$xdir$non_pic_object # A standard non-PIC object func_append non_pic_objects " $non_pic_object" if test -z "$pic_object" || test none = "$pic_object"; then arg=$non_pic_object fi else # If the PIC object exists, use it instead. # $xdir was prepended to $pic_object above. non_pic_object=$pic_object func_append non_pic_objects " $non_pic_object" fi else # Only an error if not doing a dry-run. if $opt_dry_run; then # Extract subdirectory from the argument. func_dirname "$arg" "/" "" xdir=$func_dirname_result func_lo2o "$arg" pic_object=$xdir$objdir/$func_lo2o_result non_pic_object=$xdir$func_lo2o_result func_append libobjs " $pic_object" func_append non_pic_objects " $non_pic_object" else func_fatal_error "'$arg' is not a valid libtool object" fi fi ;; 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then eval arg=\"$export_dynamic_flag_spec\" func_append compile_command " $arg" func_append finalize_command " $arg" fi oldlibs= # calculate the name of the file, without its directory func_basename "$output" outputname=$func_basename_result libobjs_save=$libobjs if test -n "$shlibpath_var"; then # get the directories listed in $shlibpath_var eval shlib_search_path=\`\$ECHO \"\$$shlibpath_var\" \| \$SED \'s/:/ /g\'\` else shlib_search_path= fi eval sys_lib_search_path=\"$sys_lib_search_path_spec\" eval sys_lib_dlsearch_path=\"$sys_lib_dlsearch_path_spec\" # Definition is injected by LT_CONFIG during libtool generation. func_munge_path_list sys_lib_dlsearch_path "$LT_SYS_LIBRARY_PATH" func_dirname "$output" "/" "" output_objdir=$func_dirname_result$objdir func_to_tool_file "$output_objdir/" tool_output_objdir=$func_to_tool_file_result # Create the object directory. func_mkdir_p "$output_objdir" # Determine the type of output case $output in "") func_fatal_help "you must specify an output file" ;; 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do case $file in *.la) ;; *) func_fatal_help "libraries can '-dlopen' only libtool libraries: $file" ;; esac done ;; prog) compile_deplibs= finalize_deplibs= alldeplibs=false newdlfiles= newdlprefiles= passes="conv scan dlopen dlpreopen link" ;; *) passes="conv" ;; esac for pass in $passes; do # The preopen pass in lib mode reverses $deplibs; put it back here # so that -L comes before libs that need it for instance... if test lib,link = "$linkmode,$pass"; then ## FIXME: Find the place where the list is rebuilt in the wrong ## order, and fix it there properly tmp_deplibs= for deplib in $deplibs; do tmp_deplibs="$deplib $tmp_deplibs" done deplibs=$tmp_deplibs fi if test lib,link = "$linkmode,$pass" || test prog,scan = "$linkmode,$pass"; then libs=$deplibs deplibs= fi if test prog = "$linkmode"; then case $pass in dlopen) libs=$dlfiles ;; dlpreopen) libs=$dlprefiles ;; link) libs="$deplibs %DEPLIBS% $dependency_libs" ;; esac fi if test lib,dlpreopen = "$linkmode,$pass"; then # Collect and forward deplibs of preopened libtool libs for lib in $dlprefiles; do # Ignore non-libtool-libs dependency_libs= func_resolve_sysroot "$lib" case $lib in *.la) func_source "$func_resolve_sysroot_result" ;; esac # Collect preopened libtool deplibs, except any this library # has declared as weak libs for deplib in $dependency_libs; do func_basename "$deplib" deplib_base=$func_basename_result case " $weak_libs " in *" $deplib_base "*) ;; *) func_append deplibs " $deplib" ;; esac done done libs=$dlprefiles fi if test dlopen = "$pass"; then # Collect dlpreopened libraries save_deplibs=$deplibs deplibs= fi for deplib in $libs; do lib= found=false case $deplib in -mt|-mthreads|-kthread|-Kthread|-pthread|-pthreads|--thread-safe \ |-threads|-fopenmp|-openmp|-mp|-xopenmp|-omp|-qsmp=*) if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else func_append compiler_flags " $deplib" if test lib = "$linkmode"; then case "$new_inherited_linker_flags " in *" $deplib "*) ;; * ) func_append new_inherited_linker_flags " $deplib" ;; esac fi fi continue ;; -l*) if test lib != "$linkmode" && test prog != "$linkmode"; then func_warning "'-l' is ignored for archives/objects" continue fi func_stripname '-l' '' "$deplib" name=$func_stripname_result if test lib = "$linkmode"; then searchdirs="$newlib_search_path $lib_search_path $compiler_lib_search_dirs $sys_lib_search_path $shlib_search_path" else searchdirs="$newlib_search_path $lib_search_path $sys_lib_search_path $shlib_search_path" fi for searchdir in $searchdirs; do for search_ext in .la $std_shrext .so .a; do # Search the libtool library lib=$searchdir/lib$name$search_ext if test -f "$lib"; then if test .la = "$search_ext"; then found=: else found=false fi break 2 fi done done if $found; then # deplib is a libtool library # If $allow_libtool_libs_with_static_runtimes && $deplib is a stdlib, # We need to do some special things here, and not later. if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $deplib "*) if func_lalib_p "$lib"; then library_names= old_library= func_source "$lib" for l in $old_library $library_names; do ll=$l done if test "X$ll" = "X$old_library"; then # only static version available found=false func_dirname "$lib" "" "." ladir=$func_dirname_result lib=$ladir/$old_library if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else deplibs="$deplib $deplibs" test lib = "$linkmode" && newdependency_libs="$deplib $newdependency_libs" fi continue fi fi ;; *) ;; esac fi else # deplib doesn't seem to be a libtool library if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else deplibs="$deplib $deplibs" test lib = "$linkmode" && newdependency_libs="$deplib $newdependency_libs" fi continue fi ;; # -l *.ltframework) if test prog,link = "$linkmode,$pass"; then compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else deplibs="$deplib $deplibs" if test lib = "$linkmode"; then case "$new_inherited_linker_flags " in *" $deplib "*) ;; * ) func_append new_inherited_linker_flags " $deplib" ;; esac fi fi continue ;; -L*) case $linkmode in lib) deplibs="$deplib $deplibs" test conv = "$pass" && continue newdependency_libs="$deplib $newdependency_libs" func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result" func_append newlib_search_path " $func_resolve_sysroot_result" ;; prog) if test conv = "$pass"; then deplibs="$deplib $deplibs" continue fi if test scan = "$pass"; then deplibs="$deplib $deplibs" else compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" fi func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result" func_append newlib_search_path " $func_resolve_sysroot_result" ;; *) func_warning "'-L' is ignored for archives/objects" ;; esac # linkmode continue ;; # -L -R*) if test link = "$pass"; then func_stripname '-R' '' "$deplib" func_resolve_sysroot "$func_stripname_result" dir=$func_resolve_sysroot_result # Make sure the xrpath contains only unique directories. case "$xrpath " in *" $dir "*) ;; *) func_append xrpath " $dir" ;; esac fi deplibs="$deplib $deplibs" continue ;; *.la) func_resolve_sysroot "$deplib" lib=$func_resolve_sysroot_result ;; *.$libext) if test conv = "$pass"; then deplibs="$deplib $deplibs" continue fi case $linkmode in lib) # Linking convenience modules into shared libraries is allowed, # but linking other static libraries is non-portable. case " $dlpreconveniencelibs " in *" $deplib "*) ;; *) valid_a_lib=false case $deplibs_check_method in match_pattern*) set dummy $deplibs_check_method; shift match_pattern_regex=`expr "$deplibs_check_method" : "$1 \(.*\)"` if eval "\$ECHO \"$deplib\"" 2>/dev/null | $SED 10q \ | $EGREP "$match_pattern_regex" > /dev/null; then valid_a_lib=: fi ;; pass_all) valid_a_lib=: ;; esac if $valid_a_lib; then echo $ECHO "*** Warning: Linking the shared library $output against the" $ECHO "*** static library $deplib is not portable!" deplibs="$deplib $deplibs" else echo $ECHO "*** Warning: Trying to link with static lib archive $deplib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because the file extensions .$libext of this argument makes me believe" echo "*** that it is just a static archive that I should not use here." fi ;; esac continue ;; prog) if test link != "$pass"; then deplibs="$deplib $deplibs" else compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" fi continue ;; esac # linkmode ;; # *.$libext *.lo | *.$objext) if test conv = "$pass"; then deplibs="$deplib $deplibs" elif test prog = "$linkmode"; then if test dlpreopen = "$pass" || test yes != "$dlopen_support" || test no = "$build_libtool_libs"; then # If there is no dlopen support or we're linking statically, # we need to preload. func_append newdlprefiles " $deplib" compile_deplibs="$deplib $compile_deplibs" finalize_deplibs="$deplib $finalize_deplibs" else func_append newdlfiles " $deplib" fi fi continue ;; %DEPLIBS%) alldeplibs=: continue ;; esac # case $deplib $found || test -f "$lib" \ || func_fatal_error "cannot find the library '$lib' or unhandled argument '$deplib'" # Check to see that this really is a libtool archive. func_lalib_unsafe_p "$lib" \ || func_fatal_error "'$lib' is not a valid libtool archive" func_dirname "$lib" "" "." ladir=$func_dirname_result dlname= dlopen= dlpreopen= libdir= library_names= old_library= inherited_linker_flags= # If the library was installed with an old release of libtool, # it will not redefine variables installed, or shouldnotlink installed=yes shouldnotlink=no avoidtemprpath= # Read the .la file func_source "$lib" # Convert "-framework foo" to "foo.ltframework" if test -n "$inherited_linker_flags"; then tmp_inherited_linker_flags=`$ECHO "$inherited_linker_flags" | $SED 's/-framework \([^ $]*\)/\1.ltframework/g'` for tmp_inherited_linker_flag in $tmp_inherited_linker_flags; do case " $new_inherited_linker_flags " in *" $tmp_inherited_linker_flag "*) ;; *) func_append new_inherited_linker_flags " $tmp_inherited_linker_flag";; esac done fi dependency_libs=`$ECHO " $dependency_libs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` if test lib,link = "$linkmode,$pass" || test prog,scan = "$linkmode,$pass" || { test prog != "$linkmode" && test lib != "$linkmode"; }; then test -n "$dlopen" && func_append dlfiles " $dlopen" test -n "$dlpreopen" && func_append dlprefiles " $dlpreopen" fi if test conv = "$pass"; then # Only check for convenience libraries deplibs="$lib $deplibs" if test -z "$libdir"; then if test -z "$old_library"; then func_fatal_error "cannot find name of link library for '$lib'" fi # It is a libtool convenience library, so add in its objects. func_append convenience " $ladir/$objdir/$old_library" func_append old_convenience " $ladir/$objdir/$old_library" elif test prog != "$linkmode" && test lib != "$linkmode"; then func_fatal_error "'$lib' is not a convenience library" fi tmp_libs= for deplib in $dependency_libs; do deplibs="$deplib $deplibs" if $opt_preserve_dup_deps; then case "$tmp_libs " in *" $deplib "*) func_append specialdeplibs " $deplib" ;; esac fi func_append tmp_libs " $deplib" done continue fi # $pass = conv # Get the name of the library we link against. linklib= if test -n "$old_library" && { test yes = "$prefer_static_libs" || test built,no = "$prefer_static_libs,$installed"; }; then linklib=$old_library else for l in $old_library $library_names; do linklib=$l done fi if test -z "$linklib"; then func_fatal_error "cannot find name of link library for '$lib'" fi # This library was specified with -dlopen. if test dlopen = "$pass"; then test -z "$libdir" \ && func_fatal_error "cannot -dlopen a convenience library: '$lib'" if test -z "$dlname" || test yes != "$dlopen_support" || test no = "$build_libtool_libs" then # If there is no dlname, no dlopen support or we're linking # statically, we need to preload. We also need to preload any # dependent libraries so libltdl's deplib preloader doesn't # bomb out in the load deplibs phase. func_append dlprefiles " $lib $dependency_libs" else func_append newdlfiles " $lib" fi continue fi # $pass = dlopen # We need an absolute path. case $ladir in [\\/]* | [A-Za-z]:[\\/]*) abs_ladir=$ladir ;; *) abs_ladir=`cd "$ladir" && pwd` if test -z "$abs_ladir"; then func_warning "cannot determine absolute directory name of '$ladir'" func_warning "passing it literally to the linker, although it might fail" abs_ladir=$ladir fi ;; esac func_basename "$lib" laname=$func_basename_result # Find the relevant object directory and library name. if test yes = "$installed"; then if test ! -f "$lt_sysroot$libdir/$linklib" && test -f "$abs_ladir/$linklib"; then func_warning "library '$lib' was moved." dir=$ladir absdir=$abs_ladir libdir=$abs_ladir else dir=$lt_sysroot$libdir absdir=$lt_sysroot$libdir fi test yes = "$hardcode_automatic" && avoidtemprpath=yes else if test ! -f "$ladir/$objdir/$linklib" && test -f "$abs_ladir/$linklib"; then dir=$ladir absdir=$abs_ladir # Remove this search path later func_append notinst_path " $abs_ladir" else dir=$ladir/$objdir absdir=$abs_ladir/$objdir # Remove this search path later func_append notinst_path " $abs_ladir" fi fi # $installed = yes func_stripname 'lib' '.la' "$laname" name=$func_stripname_result # This library was specified with -dlpreopen. if test dlpreopen = "$pass"; then if test -z "$libdir" && test prog = "$linkmode"; then func_fatal_error "only libraries may -dlpreopen a convenience library: '$lib'" fi case $host in # special handling for platforms with PE-DLLs. *cygwin* | *mingw* | *cegcc* ) # Linker will automatically link against shared library if both # static and shared are present. Therefore, ensure we extract # symbols from the import library if a shared library is present # (otherwise, the dlopen module name will be incorrect). We do # this by putting the import library name into $newdlprefiles. # We recover the dlopen module name by 'saving' the la file # name in a special purpose variable, and (later) extracting the # dlname from the la file. if test -n "$dlname"; then func_tr_sh "$dir/$linklib" eval "libfile_$func_tr_sh_result=\$abs_ladir/\$laname" func_append newdlprefiles " $dir/$linklib" else func_append newdlprefiles " $dir/$old_library" # Keep a list of preopened convenience libraries to check # that they are being used correctly in the link pass. test -z "$libdir" && \ func_append dlpreconveniencelibs " $dir/$old_library" fi ;; * ) # Prefer using a static library (so that no silly _DYNAMIC symbols # are required to link). if test -n "$old_library"; then func_append newdlprefiles " $dir/$old_library" # Keep a list of preopened convenience libraries to check # that they are being used correctly in the link pass. test -z "$libdir" && \ func_append dlpreconveniencelibs " $dir/$old_library" # Otherwise, use the dlname, so that lt_dlopen finds it. elif test -n "$dlname"; then func_append newdlprefiles " $dir/$dlname" else func_append newdlprefiles " $dir/$linklib" fi ;; esac fi # $pass = dlpreopen if test -z "$libdir"; then # Link the convenience library if test lib = "$linkmode"; then deplibs="$dir/$old_library $deplibs" elif test prog,link = "$linkmode,$pass"; then compile_deplibs="$dir/$old_library $compile_deplibs" finalize_deplibs="$dir/$old_library $finalize_deplibs" else deplibs="$lib $deplibs" # used for prog,scan pass fi continue fi if test prog = "$linkmode" && test link != "$pass"; then func_append newlib_search_path " $ladir" deplibs="$lib $deplibs" linkalldeplibs=false if test no != "$link_all_deplibs" || test -z "$library_names" || test no = "$build_libtool_libs"; then linkalldeplibs=: fi tmp_libs= for deplib in $dependency_libs; do case $deplib in -L*) func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result" func_append newlib_search_path " $func_resolve_sysroot_result" ;; esac # Need to link against all dependency_libs? if $linkalldeplibs; then deplibs="$deplib $deplibs" else # Need to hardcode shared library paths # or/and link against static libraries newdependency_libs="$deplib $newdependency_libs" fi if $opt_preserve_dup_deps; then case "$tmp_libs " in *" $deplib "*) func_append specialdeplibs " $deplib" ;; esac fi func_append tmp_libs " $deplib" done # for deplib continue fi # $linkmode = prog... if test prog,link = "$linkmode,$pass"; then if test -n "$library_names" && { { test no = "$prefer_static_libs" || test built,yes = "$prefer_static_libs,$installed"; } || test -z "$old_library"; }; then # We need to hardcode the library path if test -n "$shlibpath_var" && test -z "$avoidtemprpath"; then # Make sure the rpath contains only unique directories. case $temp_rpath: in *"$absdir:"*) ;; *) func_append temp_rpath "$absdir:" ;; esac fi # Hardcode the library path. # Skip directories that are in the system default run-time # search path. case " $sys_lib_dlsearch_path " in *" $absdir "*) ;; *) case "$compile_rpath " in *" $absdir "*) ;; *) func_append compile_rpath " $absdir" ;; esac ;; esac case " $sys_lib_dlsearch_path " in *" $libdir "*) ;; *) case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac ;; esac fi # $linkmode,$pass = prog,link... if $alldeplibs && { test pass_all = "$deplibs_check_method" || { test yes = "$build_libtool_libs" && test -n "$library_names"; }; }; then # We only need to search for static libraries continue fi fi link_static=no # Whether the deplib will be linked statically use_static_libs=$prefer_static_libs if test built = "$use_static_libs" && test yes = "$installed"; then use_static_libs=no fi if test -n "$library_names" && { test no = "$use_static_libs" || test -z "$old_library"; }; then case $host in *cygwin* | *mingw* | *cegcc* | *os2*) # No point in relinking DLLs because paths are not encoded func_append notinst_deplibs " $lib" need_relink=no ;; *) if test no = "$installed"; then func_append notinst_deplibs " $lib" need_relink=yes fi ;; esac # This is a shared library # Warn about portability, can't link against -module's on some # systems (darwin). Don't bleat about dlopened modules though! dlopenmodule= for dlpremoduletest in $dlprefiles; do if test "X$dlpremoduletest" = "X$lib"; then dlopenmodule=$dlpremoduletest break fi done if test -z "$dlopenmodule" && test yes = "$shouldnotlink" && test link = "$pass"; then echo if test prog = "$linkmode"; then $ECHO "*** Warning: Linking the executable $output against the loadable module" else $ECHO "*** Warning: Linking the shared library $output against the loadable module" fi $ECHO "*** $linklib is not portable!" fi if test lib = "$linkmode" && test yes = "$hardcode_into_libs"; then # Hardcode the library path. # Skip directories that are in the system default run-time # search path. case " $sys_lib_dlsearch_path " in *" $absdir "*) ;; *) case "$compile_rpath " in *" $absdir "*) ;; *) func_append compile_rpath " $absdir" ;; esac ;; esac case " $sys_lib_dlsearch_path " in *" $libdir "*) ;; *) case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac ;; esac fi if test -n "$old_archive_from_expsyms_cmds"; then # figure out the soname set dummy $library_names shift realname=$1 shift libname=`eval "\\$ECHO \"$libname_spec\""` # use dlname if we got it. it's perfectly good, no? if test -n "$dlname"; then soname=$dlname elif test -n "$soname_spec"; then # bleh windows case $host in *cygwin* | mingw* | *cegcc* | *os2*) func_arith $current - $age major=$func_arith_result versuffix=-$major ;; esac eval soname=\"$soname_spec\" else soname=$realname fi # Make a new name for the extract_expsyms_cmds to use soroot=$soname func_basename "$soroot" soname=$func_basename_result func_stripname 'lib' '.dll' "$soname" newlib=libimp-$func_stripname_result.a # If the library has no export list, then create one now if test -f "$output_objdir/$soname-def"; then : else func_verbose "extracting exported symbol list from '$soname'" func_execute_cmds "$extract_expsyms_cmds" 'exit $?' fi # Create $newlib if test -f "$output_objdir/$newlib"; then :; else func_verbose "generating import library for '$soname'" func_execute_cmds "$old_archive_from_expsyms_cmds" 'exit $?' fi # make sure the library variables are pointing to the new library dir=$output_objdir linklib=$newlib fi # test -n "$old_archive_from_expsyms_cmds" if test prog = "$linkmode" || test relink != "$opt_mode"; then add_shlibpath= add_dir= add= lib_linked=yes case $hardcode_action in immediate | unsupported) if test no = "$hardcode_direct"; then add=$dir/$linklib case $host in *-*-sco3.2v5.0.[024]*) add_dir=-L$dir ;; *-*-sysv4*uw2*) add_dir=-L$dir ;; *-*-sysv5OpenUNIX* | *-*-sysv5UnixWare7.[01].[10]* | \ *-*-unixware7*) add_dir=-L$dir ;; *-*-darwin* ) # if the lib is a (non-dlopened) module then we cannot # link against it, someone is ignoring the earlier warnings if /usr/bin/file -L $add 2> /dev/null | $GREP ": [^:]* bundle" >/dev/null; then if test "X$dlopenmodule" != "X$lib"; then $ECHO "*** Warning: lib $linklib is a module, not a shared library" if test -z "$old_library"; then echo echo "*** And there doesn't seem to be a static archive available" echo "*** The link will probably fail, sorry" else add=$dir/$old_library fi elif test -n "$old_library"; then add=$dir/$old_library fi fi esac elif test no = "$hardcode_minus_L"; then case $host in *-*-sunos*) add_shlibpath=$dir ;; esac add_dir=-L$dir add=-l$name elif test no = "$hardcode_shlibpath_var"; then add_shlibpath=$dir add=-l$name else lib_linked=no fi ;; relink) if test yes = "$hardcode_direct" && test no = "$hardcode_direct_absolute"; then add=$dir/$linklib elif test yes = "$hardcode_minus_L"; then add_dir=-L$absdir # Try looking first in the location we're being installed to. if test -n "$inst_prefix_dir"; then case $libdir in [\\/]*) func_append add_dir " -L$inst_prefix_dir$libdir" ;; esac fi add=-l$name elif test yes = "$hardcode_shlibpath_var"; then add_shlibpath=$dir add=-l$name else lib_linked=no fi ;; *) lib_linked=no ;; esac if test yes != "$lib_linked"; then func_fatal_configuration "unsupported hardcode properties" fi if test -n "$add_shlibpath"; then case :$compile_shlibpath: in *":$add_shlibpath:"*) ;; *) func_append compile_shlibpath "$add_shlibpath:" ;; esac fi if test prog = "$linkmode"; then test -n "$add_dir" && compile_deplibs="$add_dir $compile_deplibs" test -n "$add" && compile_deplibs="$add $compile_deplibs" else test -n "$add_dir" && deplibs="$add_dir $deplibs" test -n "$add" && deplibs="$add $deplibs" if test yes != "$hardcode_direct" && test yes != "$hardcode_minus_L" && test yes = "$hardcode_shlibpath_var"; then case :$finalize_shlibpath: in *":$libdir:"*) ;; *) func_append finalize_shlibpath "$libdir:" ;; esac fi fi fi if test prog = "$linkmode" || test relink = "$opt_mode"; then add_shlibpath= add_dir= add= # Finalize command for both is simple: just hardcode it. if test yes = "$hardcode_direct" && test no = "$hardcode_direct_absolute"; then add=$libdir/$linklib elif test yes = "$hardcode_minus_L"; then add_dir=-L$libdir add=-l$name elif test yes = "$hardcode_shlibpath_var"; then case :$finalize_shlibpath: in *":$libdir:"*) ;; *) func_append finalize_shlibpath "$libdir:" ;; esac add=-l$name elif test yes = "$hardcode_automatic"; then if test -n "$inst_prefix_dir" && test -f "$inst_prefix_dir$libdir/$linklib"; then add=$inst_prefix_dir$libdir/$linklib else add=$libdir/$linklib fi else # We cannot seem to hardcode it, guess we'll fake it. add_dir=-L$libdir # Try looking first in the location we're being installed to. if test -n "$inst_prefix_dir"; then case $libdir in [\\/]*) func_append add_dir " -L$inst_prefix_dir$libdir" ;; esac fi add=-l$name fi if test prog = "$linkmode"; then test -n "$add_dir" && finalize_deplibs="$add_dir $finalize_deplibs" test -n "$add" && finalize_deplibs="$add $finalize_deplibs" else test -n "$add_dir" && deplibs="$add_dir $deplibs" test -n "$add" && deplibs="$add $deplibs" fi fi elif test prog = "$linkmode"; then # Here we assume that one of hardcode_direct or hardcode_minus_L # is not unsupported. This is valid on all known static and # shared platforms. if test unsupported != "$hardcode_direct"; then test -n "$old_library" && linklib=$old_library compile_deplibs="$dir/$linklib $compile_deplibs" finalize_deplibs="$dir/$linklib $finalize_deplibs" else compile_deplibs="-l$name -L$dir $compile_deplibs" finalize_deplibs="-l$name -L$dir $finalize_deplibs" fi elif test yes = "$build_libtool_libs"; then # Not a shared library if test pass_all != "$deplibs_check_method"; then # We're trying link a shared library against a static one # but the system doesn't support it. # Just print a warning and add the library to dependency_libs so # that the program can be linked against the static library. echo $ECHO "*** Warning: This system cannot link to static lib archive $lib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have." if test yes = "$module"; then echo "*** But as you try to build a module library, libtool will still create " echo "*** a static module, that should work as long as the dlopening application" echo "*** is linked with the -dlopen flag to resolve symbols at runtime." if test -z "$global_symbol_pipe"; then echo echo "*** However, this would only work if libtool was able to extract symbol" echo "*** lists from a program, using 'nm' or equivalent, but libtool could" echo "*** not find such a program. So, this module is probably useless." echo "*** 'nm' from GNU binutils and a full rebuild may help." fi if test no = "$build_old_libs"; then build_libtool_libs=module build_old_libs=yes else build_libtool_libs=no fi fi else deplibs="$dir/$old_library $deplibs" link_static=yes fi fi # link shared/static library? if test lib = "$linkmode"; then if test -n "$dependency_libs" && { test yes != "$hardcode_into_libs" || test yes = "$build_old_libs" || test yes = "$link_static"; }; then # Extract -R from dependency_libs temp_deplibs= for libdir in $dependency_libs; do case $libdir in -R*) func_stripname '-R' '' "$libdir" temp_xrpath=$func_stripname_result case " $xrpath " in *" $temp_xrpath "*) ;; *) func_append xrpath " $temp_xrpath";; esac;; *) func_append temp_deplibs " $libdir";; esac done dependency_libs=$temp_deplibs fi func_append newlib_search_path " $absdir" # Link against this library test no = "$link_static" && newdependency_libs="$abs_ladir/$laname $newdependency_libs" # ... and its dependency_libs tmp_libs= for deplib in $dependency_libs; do newdependency_libs="$deplib $newdependency_libs" case $deplib in -L*) func_stripname '-L' '' "$deplib" func_resolve_sysroot "$func_stripname_result";; *) func_resolve_sysroot "$deplib" ;; esac if $opt_preserve_dup_deps; then case "$tmp_libs " in *" $func_resolve_sysroot_result "*) func_append specialdeplibs " $func_resolve_sysroot_result" ;; esac fi func_append tmp_libs " $func_resolve_sysroot_result" done if test no != "$link_all_deplibs"; then # Add the search paths of all dependency libraries for deplib in $dependency_libs; do path= case $deplib in -L*) path=$deplib ;; *.la) func_resolve_sysroot "$deplib" deplib=$func_resolve_sysroot_result func_dirname "$deplib" "" "." dir=$func_dirname_result # We need an absolute path. case $dir in [\\/]* | [A-Za-z]:[\\/]*) absdir=$dir ;; *) absdir=`cd "$dir" && pwd` if test -z "$absdir"; then func_warning "cannot determine absolute directory name of '$dir'" absdir=$dir fi ;; esac if $GREP "^installed=no" $deplib > /dev/null; then case $host in *-*-darwin*) depdepl= eval deplibrary_names=`$SED -n -e 's/^library_names=\(.*\)$/\1/p' $deplib` if test -n "$deplibrary_names"; then for tmp in $deplibrary_names; do depdepl=$tmp done if test -f "$absdir/$objdir/$depdepl"; then depdepl=$absdir/$objdir/$depdepl darwin_install_name=`$OTOOL -L $depdepl | awk '{if (NR == 2) {print $1;exit}}'` if test -z "$darwin_install_name"; then darwin_install_name=`$OTOOL64 -L $depdepl | awk '{if (NR == 2) {print $1;exit}}'` fi func_append compiler_flags " $wl-dylib_file $wl$darwin_install_name:$depdepl" func_append linker_flags " -dylib_file $darwin_install_name:$depdepl" path= fi fi ;; *) path=-L$absdir/$objdir ;; esac else eval libdir=`$SED -n -e 's/^libdir=\(.*\)$/\1/p' $deplib` test -z "$libdir" && \ func_fatal_error "'$deplib' is not a valid libtool archive" test "$absdir" != "$libdir" && \ func_warning "'$deplib' seems to be moved" path=-L$absdir fi ;; esac case " $deplibs " in *" $path "*) ;; *) deplibs="$path $deplibs" ;; esac done fi # link_all_deplibs != no fi # linkmode = lib done # for deplib in $libs if test link = "$pass"; then if test prog = "$linkmode"; then compile_deplibs="$new_inherited_linker_flags $compile_deplibs" finalize_deplibs="$new_inherited_linker_flags $finalize_deplibs" else compiler_flags="$compiler_flags "`$ECHO " $new_inherited_linker_flags" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` fi fi dependency_libs=$newdependency_libs if test dlpreopen = "$pass"; then # Link the dlpreopened libraries before other libraries for deplib in $save_deplibs; do deplibs="$deplib $deplibs" done fi if test dlopen != "$pass"; then test conv = "$pass" || { # Make sure lib_search_path contains only unique directories. lib_search_path= for dir in $newlib_search_path; do case "$lib_search_path " in *" $dir "*) ;; *) func_append lib_search_path " $dir" ;; esac done newlib_search_path= } if test prog,link = "$linkmode,$pass"; then vars="compile_deplibs finalize_deplibs" else vars=deplibs fi for var in $vars dependency_libs; do # Add libraries to $var in reverse order eval tmp_libs=\"\$$var\" new_libs= for deplib in $tmp_libs; do # FIXME: Pedantically, this is the right thing to do, so # that some nasty dependency loop isn't accidentally # broken: #new_libs="$deplib $new_libs" # Pragmatically, this seems to cause very few problems in # practice: case $deplib in -L*) new_libs="$deplib $new_libs" ;; -R*) ;; *) # And here is the reason: when a library appears more # than once as an explicit dependence of a library, or # is implicitly linked in more than once by the # compiler, it is considered special, and multiple # occurrences thereof are not removed. Compare this # with having the same library being listed as a # dependency of multiple other libraries: in this case, # we know (pedantically, we assume) the library does not # need to be listed more than once, so we keep only the # last copy. This is not always right, but it is rare # enough that we require users that really mean to play # such unportable linking tricks to link the library # using -Wl,-lname, so that libtool does not consider it # for duplicate removal. case " $specialdeplibs " in *" $deplib "*) new_libs="$deplib $new_libs" ;; *) case " $new_libs " in *" $deplib "*) ;; *) new_libs="$deplib $new_libs" ;; esac ;; esac ;; esac done tmp_libs= for deplib in $new_libs; do case $deplib in -L*) case " $tmp_libs " in *" $deplib "*) ;; *) func_append tmp_libs " $deplib" ;; esac ;; *) func_append tmp_libs " $deplib" ;; esac done eval $var=\"$tmp_libs\" done # for var fi # Add Sun CC postdeps if required: test CXX = "$tagname" && { case $host_os in linux*) case `$CC -V 2>&1 | sed 5q` in *Sun\ C*) # Sun C++ 5.9 func_suncc_cstd_abi if test no != "$suncc_use_cstd_abi"; then func_append postdeps ' -library=Cstd -library=Crun' fi ;; esac ;; solaris*) func_cc_basename "$CC" case $func_cc_basename_result in CC* | sunCC*) func_suncc_cstd_abi if test no != "$suncc_use_cstd_abi"; then func_append postdeps ' -library=Cstd -library=Crun' fi ;; esac ;; esac } # Last step: remove runtime libs from dependency_libs # (they stay in deplibs) tmp_libs= for i in $dependency_libs; do case " $predeps $postdeps $compiler_lib_search_path " in *" $i "*) i= ;; esac if test -n "$i"; then func_append tmp_libs " $i" fi done dependency_libs=$tmp_libs done # for pass if test prog = "$linkmode"; then dlfiles=$newdlfiles fi if test prog = "$linkmode" || test lib = "$linkmode"; then dlprefiles=$newdlprefiles fi case $linkmode in oldlib) if test -n "$dlfiles$dlprefiles" || test no != "$dlself"; then func_warning "'-dlopen' is ignored for archives" fi case " $deplibs" in *\ -l* | *\ -L*) func_warning "'-l' and '-L' are ignored for archives" ;; esac test -n "$rpath" && \ func_warning "'-rpath' is ignored for archives" test -n "$xrpath" && \ func_warning "'-R' is ignored for archives" test -n "$vinfo" && \ func_warning "'-version-info/-version-number' is ignored for archives" test -n "$release" && \ func_warning "'-release' is ignored for archives" test -n "$export_symbols$export_symbols_regex" && \ func_warning "'-export-symbols' is ignored for archives" # Now set the variables for building old libraries. build_libtool_libs=no oldlibs=$output func_append objs "$old_deplibs" ;; lib) # Make sure we only generate libraries of the form 'libNAME.la'. case $outputname in lib*) func_stripname 'lib' '.la' "$outputname" name=$func_stripname_result eval shared_ext=\"$shrext_cmds\" eval libname=\"$libname_spec\" ;; *) test no = "$module" \ && func_fatal_help "libtool library '$output' must begin with 'lib'" if test no != "$need_lib_prefix"; then # Add the "lib" prefix for modules if required func_stripname '' '.la' "$outputname" name=$func_stripname_result eval shared_ext=\"$shrext_cmds\" eval libname=\"$libname_spec\" else func_stripname '' '.la' "$outputname" libname=$func_stripname_result fi ;; esac if test -n "$objs"; then if test pass_all != "$deplibs_check_method"; then func_fatal_error "cannot build libtool library '$output' from non-libtool objects on this host:$objs" else echo $ECHO "*** Warning: Linking the shared library $output against the non-libtool" $ECHO "*** objects $objs is not portable!" func_append libobjs " $objs" fi fi test no = "$dlself" \ || func_warning "'-dlopen self' is ignored for libtool libraries" set dummy $rpath shift test 1 -lt "$#" \ && func_warning "ignoring multiple '-rpath's for a libtool library" install_libdir=$1 oldlibs= if test -z "$rpath"; then if test yes = "$build_libtool_libs"; then # Building a libtool convenience library. # Some compilers have problems with a '.al' extension so # convenience libraries should have the same extension an # archive normally would. oldlibs="$output_objdir/$libname.$libext $oldlibs" build_libtool_libs=convenience build_old_libs=yes fi test -n "$vinfo" && \ func_warning "'-version-info/-version-number' is ignored for convenience libraries" test -n "$release" && \ func_warning "'-release' is ignored for convenience libraries" else # Parse the version information argument. save_ifs=$IFS; IFS=: set dummy $vinfo 0 0 0 shift IFS=$save_ifs test -n "$7" && \ func_fatal_help "too many parameters to '-version-info'" # convert absolute version numbers to libtool ages # this retains compatibility with .la files and attempts # to make the code below a bit more comprehensible case $vinfo_number in yes) number_major=$1 number_minor=$2 number_revision=$3 # # There are really only two kinds -- those that # use the current revision as the major version # and those that subtract age and use age as # a minor version. But, then there is irix # that has an extra 1 added just for fun # case $version_type in # correct linux to gnu/linux during the next big refactor darwin|freebsd-elf|linux|osf|windows|none) func_arith $number_major + $number_minor current=$func_arith_result age=$number_minor revision=$number_revision ;; freebsd-aout|qnx|sunos) current=$number_major revision=$number_minor age=0 ;; irix|nonstopux) func_arith $number_major + $number_minor current=$func_arith_result age=$number_minor revision=$number_minor lt_irix_increment=no ;; esac ;; no) current=$1 revision=$2 age=$3 ;; esac # Check that each of the things are valid numbers. case $current in 0|[1-9]|[1-9][0-9]|[1-9][0-9][0-9]|[1-9][0-9][0-9][0-9]|[1-9][0-9][0-9][0-9][0-9]) ;; *) func_error "CURRENT '$current' must be a nonnegative integer" func_fatal_error "'$vinfo' is not valid version information" ;; esac case $revision in 0|[1-9]|[1-9][0-9]|[1-9][0-9][0-9]|[1-9][0-9][0-9][0-9]|[1-9][0-9][0-9][0-9][0-9]) ;; *) func_error "REVISION '$revision' must be a nonnegative integer" func_fatal_error "'$vinfo' is not valid version information" ;; esac case $age in 0|[1-9]|[1-9][0-9]|[1-9][0-9][0-9]|[1-9][0-9][0-9][0-9]|[1-9][0-9][0-9][0-9][0-9]) ;; *) func_error "AGE '$age' must be a nonnegative integer" func_fatal_error "'$vinfo' is not valid version information" ;; esac if test "$age" -gt "$current"; then func_error "AGE '$age' is greater than the current interface number '$current'" func_fatal_error "'$vinfo' is not valid version information" fi # Calculate the version variables. major= versuffix= verstring= case $version_type in none) ;; darwin) # Like Linux, but with the current version available in # verstring for coding it into the library header func_arith $current - $age major=.$func_arith_result versuffix=$major.$age.$revision # Darwin ld doesn't like 0 for these options... func_arith $current + 1 minor_current=$func_arith_result xlcverstring="$wl-compatibility_version $wl$minor_current $wl-current_version $wl$minor_current.$revision" verstring="-compatibility_version $minor_current -current_version $minor_current.$revision" # On Darwin other compilers case $CC in nagfor*) verstring="$wl-compatibility_version $wl$minor_current $wl-current_version $wl$minor_current.$revision" ;; *) verstring="-compatibility_version $minor_current -current_version $minor_current.$revision" ;; esac ;; freebsd-aout) major=.$current versuffix=.$current.$revision ;; freebsd-elf) func_arith $current - $age major=.$func_arith_result versuffix=$major.$age.$revision ;; irix | nonstopux) if test no = "$lt_irix_increment"; then func_arith $current - $age else func_arith $current - $age + 1 fi major=$func_arith_result case $version_type in nonstopux) verstring_prefix=nonstopux ;; *) verstring_prefix=sgi ;; esac verstring=$verstring_prefix$major.$revision # Add in all the interfaces that we are compatible with. loop=$revision while test 0 -ne "$loop"; do func_arith $revision - $loop iface=$func_arith_result func_arith $loop - 1 loop=$func_arith_result verstring=$verstring_prefix$major.$iface:$verstring done # Before this point, $major must not contain '.'. major=.$major versuffix=$major.$revision ;; linux) # correct to gnu/linux during the next big refactor func_arith $current - $age major=.$func_arith_result versuffix=$major.$age.$revision ;; osf) func_arith $current - $age major=.$func_arith_result versuffix=.$current.$age.$revision verstring=$current.$age.$revision # Add in all the interfaces that we are compatible with. loop=$age while test 0 -ne "$loop"; do func_arith $current - $loop iface=$func_arith_result func_arith $loop - 1 loop=$func_arith_result verstring=$verstring:$iface.0 done # Make executables depend on our current version. func_append verstring ":$current.0" ;; qnx) major=.$current versuffix=.$current ;; sco) major=.$current versuffix=.$current ;; sunos) major=.$current versuffix=.$current.$revision ;; windows) # Use '-' rather than '.', since we only want one # extension on DOS 8.3 file systems. func_arith $current - $age major=$func_arith_result versuffix=-$major ;; *) func_fatal_configuration "unknown library version type '$version_type'" ;; esac # Clear the version info if we defaulted, and they specified a release. if test -z "$vinfo" && test -n "$release"; then major= case $version_type in darwin) # we can't check for "0.0" in archive_cmds due to quoting # problems, so we reset it completely verstring= ;; *) verstring=0.0 ;; esac if test no = "$need_version"; then versuffix= else versuffix=.0.0 fi fi # Remove version info from name if versioning should be avoided if test yes,no = "$avoid_version,$need_version"; then major= versuffix= verstring= fi # Check to see if the archive will have undefined symbols. if test yes = "$allow_undefined"; then if test unsupported = "$allow_undefined_flag"; then if test yes = "$build_old_libs"; then func_warning "undefined symbols not allowed in $host shared libraries; building static only" build_libtool_libs=no else func_fatal_error "can't build $host shared library unless -no-undefined is specified" fi fi else # Don't allow undefined symbols. allow_undefined_flag=$no_undefined_flag fi fi func_generate_dlsyms "$libname" "$libname" : func_append libobjs " $symfileobj" test " " = "$libobjs" && libobjs= if test relink != "$opt_mode"; then # Remove our outputs, but don't remove object files since they # may have been created when compiling PIC objects. removelist= tempremovelist=`$ECHO "$output_objdir/*"` for p in $tempremovelist; do case $p in *.$objext | *.gcno) ;; $output_objdir/$outputname | $output_objdir/$libname.* | $output_objdir/$libname$release.*) if test -n "$precious_files_regex"; then if $ECHO "$p" | $EGREP -e "$precious_files_regex" >/dev/null 2>&1 then continue fi fi func_append removelist " $p" ;; *) ;; esac done test -n "$removelist" && \ func_show_eval "${RM}r \$removelist" fi # Now set the variables for building old libraries. if test yes = "$build_old_libs" && test convenience != "$build_libtool_libs"; then func_append oldlibs " $output_objdir/$libname.$libext" # Transform .lo files to .o files. oldobjs="$objs "`$ECHO "$libobjs" | $SP2NL | $SED "/\.$libext$/d; $lo2o" | $NL2SP` fi # Eliminate all temporary directories. #for path in $notinst_path; do # lib_search_path=`$ECHO "$lib_search_path " | $SED "s% $path % %g"` # deplibs=`$ECHO "$deplibs " | $SED "s% -L$path % %g"` # dependency_libs=`$ECHO "$dependency_libs " | $SED "s% -L$path % %g"` #done if test -n "$xrpath"; then # If the user specified any rpath flags, then add them. temp_xrpath= for libdir in $xrpath; do func_replace_sysroot "$libdir" func_append temp_xrpath " -R$func_replace_sysroot_result" case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac done if test yes != "$hardcode_into_libs" || test yes = "$build_old_libs"; then dependency_libs="$temp_xrpath $dependency_libs" fi fi # Make sure dlfiles contains only unique files that won't be dlpreopened old_dlfiles=$dlfiles dlfiles= for lib in $old_dlfiles; do case " $dlprefiles $dlfiles " in *" $lib "*) ;; *) func_append dlfiles " $lib" ;; esac done # Make sure dlprefiles contains only unique files old_dlprefiles=$dlprefiles dlprefiles= for lib in $old_dlprefiles; do case "$dlprefiles " in *" $lib "*) ;; *) func_append dlprefiles " $lib" ;; esac done if test yes = "$build_libtool_libs"; then if test -n "$rpath"; then case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-os2* | *-*-beos* | *-cegcc* | *-*-haiku*) # these systems don't actually have a c library (as such)! ;; *-*-rhapsody* | *-*-darwin1.[012]) # Rhapsody C library is in the System framework func_append deplibs " System.ltframework" ;; *-*-netbsd*) # Don't link with libc until the a.out ld.so is fixed. ;; *-*-openbsd* | *-*-freebsd* | *-*-dragonfly*) # Do not include libc due to us having libc/libc_r. ;; *-*-sco3.2v5* | *-*-sco5v6*) # Causes problems with __ctype ;; *-*-sysv4.2uw2* | *-*-sysv5* | *-*-unixware* | *-*-OpenUNIX*) # Compiler inserts libc in the correct place for threads to work ;; *) # Add libc to deplibs on all other systems if necessary. if test yes = "$build_libtool_need_lc"; then func_append deplibs " -lc" fi ;; esac fi # Transform deplibs into only deplibs that can be linked in shared. name_save=$name libname_save=$libname release_save=$release versuffix_save=$versuffix major_save=$major # I'm not sure if I'm treating the release correctly. I think # release should show up in the -l (ie -lgmp5) so we don't want to # add it in twice. Is that correct? release= versuffix= major= newdeplibs= droppeddeps=no case $deplibs_check_method in pass_all) # Don't check for shared/static. Everything works. # This might be a little naive. We might want to check # whether the library exists or not. But this is on # osf3 & osf4 and I'm not really sure... Just # implementing what was already the behavior. newdeplibs=$deplibs ;; test_compile) # This code stresses the "libraries are programs" paradigm to its # limits. Maybe even breaks it. We compile a program, linking it # against the deplibs as a proxy for the library. Then we can check # whether they linked in statically or dynamically with ldd. $opt_dry_run || $RM conftest.c cat > conftest.c <<EOF int main() { return 0; } EOF $opt_dry_run || $RM conftest if $LTCC $LTCFLAGS -o conftest conftest.c $deplibs; then ldd_output=`ldd conftest` for i in $deplibs; do case $i in -l*) func_stripname -l '' "$i" name=$func_stripname_result if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $i "*) func_append newdeplibs " $i" i= ;; esac fi if test -n "$i"; then libname=`eval "\\$ECHO \"$libname_spec\""` deplib_matches=`eval "\\$ECHO \"$library_names_spec\""` set dummy $deplib_matches; shift deplib_match=$1 if test `expr "$ldd_output" : ".*$deplib_match"` -ne 0; then func_append newdeplibs " $i" else droppeddeps=yes echo $ECHO "*** Warning: dynamic linker does not accept needed library $i." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which I believe you do not have" echo "*** because a test_compile did reveal that the linker did not use it for" echo "*** its dynamic dependency list that programs get resolved with at runtime." fi fi ;; *) func_append newdeplibs " $i" ;; esac done else # Error occurred in the first compile. Let's try to salvage # the situation: Compile a separate program for each library. for i in $deplibs; do case $i in -l*) func_stripname -l '' "$i" name=$func_stripname_result $opt_dry_run || $RM conftest if $LTCC $LTCFLAGS -o conftest conftest.c $i; then ldd_output=`ldd conftest` if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $i "*) func_append newdeplibs " $i" i= ;; esac fi if test -n "$i"; then libname=`eval "\\$ECHO \"$libname_spec\""` deplib_matches=`eval "\\$ECHO \"$library_names_spec\""` set dummy $deplib_matches; shift deplib_match=$1 if test `expr "$ldd_output" : ".*$deplib_match"` -ne 0; then func_append newdeplibs " $i" else droppeddeps=yes echo $ECHO "*** Warning: dynamic linker does not accept needed library $i." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because a test_compile did reveal that the linker did not use this one" echo "*** as a dynamic dependency that programs can get resolved with at runtime." fi fi else droppeddeps=yes echo $ECHO "*** Warning! Library $i is needed by this library but I was not able to" echo "*** make it link in! You will probably need to install it or some" echo "*** library that it depends on before this library will be fully" echo "*** functional. Installing it before continuing would be even better." fi ;; *) func_append newdeplibs " $i" ;; esac done fi ;; file_magic*) set dummy $deplibs_check_method; shift file_magic_regex=`expr "$deplibs_check_method" : "$1 \(.*\)"` for a_deplib in $deplibs; do case $a_deplib in -l*) func_stripname -l '' "$a_deplib" name=$func_stripname_result if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $a_deplib "*) func_append newdeplibs " $a_deplib" a_deplib= ;; esac fi if test -n "$a_deplib"; then libname=`eval "\\$ECHO \"$libname_spec\""` if test -n "$file_magic_glob"; then libnameglob=`func_echo_all "$libname" | $SED -e $file_magic_glob` else libnameglob=$libname fi test yes = "$want_nocaseglob" && nocaseglob=`shopt -p nocaseglob` for i in $lib_search_path $sys_lib_search_path $shlib_search_path; do if test yes = "$want_nocaseglob"; then shopt -s nocaseglob potential_libs=`ls $i/$libnameglob[.-]* 2>/dev/null` $nocaseglob else potential_libs=`ls $i/$libnameglob[.-]* 2>/dev/null` fi for potent_lib in $potential_libs; do # Follow soft links. if ls -lLd "$potent_lib" 2>/dev/null | $GREP " -> " >/dev/null; then continue fi # The statement above tries to avoid entering an # endless loop below, in case of cyclic links. # We might still enter an endless loop, since a link # loop can be closed while we follow links, # but so what? potlib=$potent_lib while test -h "$potlib" 2>/dev/null; do potliblink=`ls -ld $potlib | $SED 's/.* -> //'` case $potliblink in [\\/]* | [A-Za-z]:[\\/]*) potlib=$potliblink;; *) potlib=`$ECHO "$potlib" | $SED 's|[^/]*$||'`"$potliblink";; esac done if eval $file_magic_cmd \"\$potlib\" 2>/dev/null | $SED -e 10q | $EGREP "$file_magic_regex" > /dev/null; then func_append newdeplibs " $a_deplib" a_deplib= break 2 fi done done fi if test -n "$a_deplib"; then droppeddeps=yes echo $ECHO "*** Warning: linker path does not have real file for library $a_deplib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because I did check the linker path looking for a file starting" if test -z "$potlib"; then $ECHO "*** with $libname but no candidates were found. (...for file magic test)" else $ECHO "*** with $libname and none of the candidates passed a file format test" $ECHO "*** using a file magic. Last file checked: $potlib" fi fi ;; *) # Add a -L argument. func_append newdeplibs " $a_deplib" ;; esac done # Gone through all deplibs. ;; match_pattern*) set dummy $deplibs_check_method; shift match_pattern_regex=`expr "$deplibs_check_method" : "$1 \(.*\)"` for a_deplib in $deplibs; do case $a_deplib in -l*) func_stripname -l '' "$a_deplib" name=$func_stripname_result if test yes = "$allow_libtool_libs_with_static_runtimes"; then case " $predeps $postdeps " in *" $a_deplib "*) func_append newdeplibs " $a_deplib" a_deplib= ;; esac fi if test -n "$a_deplib"; then libname=`eval "\\$ECHO \"$libname_spec\""` for i in $lib_search_path $sys_lib_search_path $shlib_search_path; do potential_libs=`ls $i/$libname[.-]* 2>/dev/null` for potent_lib in $potential_libs; do potlib=$potent_lib # see symlink-check above in file_magic test if eval "\$ECHO \"$potent_lib\"" 2>/dev/null | $SED 10q | \ $EGREP "$match_pattern_regex" > /dev/null; then func_append newdeplibs " $a_deplib" a_deplib= break 2 fi done done fi if test -n "$a_deplib"; then droppeddeps=yes echo $ECHO "*** Warning: linker path does not have real file for library $a_deplib." echo "*** I have the capability to make that library automatically link in when" echo "*** you link to this library. But I can only do this if you have a" echo "*** shared version of the library, which you do not appear to have" echo "*** because I did check the linker path looking for a file starting" if test -z "$potlib"; then $ECHO "*** with $libname but no candidates were found. (...for regex pattern test)" else $ECHO "*** with $libname and none of the candidates passed a file format test" $ECHO "*** using a regex pattern. Last file checked: $potlib" fi fi ;; *) # Add a -L argument. func_append newdeplibs " $a_deplib" ;; esac done # Gone through all deplibs. ;; none | unknown | *) newdeplibs= tmp_deplibs=`$ECHO " $deplibs" | $SED 's/ -lc$//; s/ -[LR][^ ]*//g'` if test yes = "$allow_libtool_libs_with_static_runtimes"; then for i in $predeps $postdeps; do # can't use Xsed below, because $i might contain '/' tmp_deplibs=`$ECHO " $tmp_deplibs" | $SED "s|$i||"` done fi case $tmp_deplibs in *[!\ \ ]*) echo if test none = "$deplibs_check_method"; then echo "*** Warning: inter-library dependencies are not supported in this platform." else echo "*** Warning: inter-library dependencies are not known to be supported." fi echo "*** All declared inter-library dependencies are being dropped." droppeddeps=yes ;; esac ;; esac versuffix=$versuffix_save major=$major_save release=$release_save libname=$libname_save name=$name_save case $host in *-*-rhapsody* | *-*-darwin1.[012]) # On Rhapsody replace the C library with the System framework newdeplibs=`$ECHO " $newdeplibs" | $SED 's/ -lc / System.ltframework /'` ;; esac if test yes = "$droppeddeps"; then if test yes = "$module"; then echo echo "*** Warning: libtool could not satisfy all declared inter-library" $ECHO "*** dependencies of module $libname. Therefore, libtool will create" echo "*** a static module, that should work as long as the dlopening" echo "*** application is linked with the -dlopen flag." if test -z "$global_symbol_pipe"; then echo echo "*** However, this would only work if libtool was able to extract symbol" echo "*** lists from a program, using 'nm' or equivalent, but libtool could" echo "*** not find such a program. So, this module is probably useless." echo "*** 'nm' from GNU binutils and a full rebuild may help." fi if test no = "$build_old_libs"; then oldlibs=$output_objdir/$libname.$libext build_libtool_libs=module build_old_libs=yes else build_libtool_libs=no fi else echo "*** The inter-library dependencies that have been dropped here will be" echo "*** automatically added whenever a program is linked with this library" echo "*** or is declared to -dlopen it." if test no = "$allow_undefined"; then echo echo "*** Since this library must not contain undefined symbols," echo "*** because either the platform does not support them or" echo "*** it was explicitly requested with -no-undefined," echo "*** libtool will only create a static version of it." if test no = "$build_old_libs"; then oldlibs=$output_objdir/$libname.$libext build_libtool_libs=module build_old_libs=yes else build_libtool_libs=no fi fi fi fi # Done checking deplibs! deplibs=$newdeplibs fi # Time to change all our "foo.ltframework" stuff back to "-framework foo" case $host in *-*-darwin*) newdeplibs=`$ECHO " $newdeplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` new_inherited_linker_flags=`$ECHO " $new_inherited_linker_flags" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` deplibs=`$ECHO " $deplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` ;; esac # move library search paths that coincide with paths to not yet # installed libraries to the beginning of the library search list new_libs= for path in $notinst_path; do case " $new_libs " in *" -L$path/$objdir "*) ;; *) case " $deplibs " in *" -L$path/$objdir "*) func_append new_libs " -L$path/$objdir" ;; esac ;; esac done for deplib in $deplibs; do case $deplib in -L*) case " $new_libs " in *" $deplib "*) ;; *) func_append new_libs " $deplib" ;; esac ;; *) func_append new_libs " $deplib" ;; esac done deplibs=$new_libs # All the library-specific variables (install_libdir is set above). library_names= old_library= dlname= # Test again, we may have decided not to build it any more if test yes = "$build_libtool_libs"; then # Remove $wl instances when linking with ld. # FIXME: should test the right _cmds variable. case $archive_cmds in *\$LD\ *) wl= ;; esac if test yes = "$hardcode_into_libs"; then # Hardcode the library paths hardcode_libdirs= dep_rpath= rpath=$finalize_rpath test relink = "$opt_mode" || rpath=$compile_rpath$rpath for libdir in $rpath; do if test -n "$hardcode_libdir_flag_spec"; then if test -n "$hardcode_libdir_separator"; then func_replace_sysroot "$libdir" libdir=$func_replace_sysroot_result if test -z "$hardcode_libdirs"; then hardcode_libdirs=$libdir else # Just accumulate the unique libdirs. case $hardcode_libdir_separator$hardcode_libdirs$hardcode_libdir_separator in *"$hardcode_libdir_separator$libdir$hardcode_libdir_separator"*) ;; *) func_append hardcode_libdirs "$hardcode_libdir_separator$libdir" ;; esac fi else eval flag=\"$hardcode_libdir_flag_spec\" func_append dep_rpath " $flag" fi elif test -n "$runpath_var"; then case "$perm_rpath " in *" $libdir "*) ;; *) func_append perm_rpath " $libdir" ;; esac fi done # Substitute the hardcoded libdirs into the rpath. if test -n "$hardcode_libdir_separator" && test -n "$hardcode_libdirs"; then libdir=$hardcode_libdirs eval "dep_rpath=\"$hardcode_libdir_flag_spec\"" fi if test -n "$runpath_var" && test -n "$perm_rpath"; then # We should set the runpath_var. rpath= for dir in $perm_rpath; do func_append rpath "$dir:" done eval "$runpath_var='$rpath\$$runpath_var'; export $runpath_var" fi test -n "$dep_rpath" && deplibs="$dep_rpath $deplibs" fi shlibpath=$finalize_shlibpath test relink = "$opt_mode" || shlibpath=$compile_shlibpath$shlibpath if test -n "$shlibpath"; then eval "$shlibpath_var='$shlibpath\$$shlibpath_var'; export $shlibpath_var" fi # Get the real and link names of the library. eval shared_ext=\"$shrext_cmds\" eval library_names=\"$library_names_spec\" set dummy $library_names shift realname=$1 shift if test -n "$soname_spec"; then eval soname=\"$soname_spec\" else soname=$realname fi if test -z "$dlname"; then dlname=$soname fi lib=$output_objdir/$realname linknames= for link do func_append linknames " $link" done # Use standard objects if they are pic test -z "$pic_flag" && libobjs=`$ECHO "$libobjs" | $SP2NL | $SED "$lo2o" | $NL2SP` test "X$libobjs" = "X " && libobjs= delfiles= if test -n "$export_symbols" && test -n "$include_expsyms"; then $opt_dry_run || cp "$export_symbols" "$output_objdir/$libname.uexp" export_symbols=$output_objdir/$libname.uexp func_append delfiles " $export_symbols" fi orig_export_symbols= case $host_os in cygwin* | mingw* | cegcc*) if test -n "$export_symbols" && test -z "$export_symbols_regex"; then # exporting using user supplied symfile func_dll_def_p "$export_symbols" || { # and it's NOT already a .def file. Must figure out # which of the given symbols are data symbols and tag # them as such. So, trigger use of export_symbols_cmds. # export_symbols gets reassigned inside the "prepare # the list of exported symbols" if statement, so the # include_expsyms logic still works. orig_export_symbols=$export_symbols export_symbols= always_export_symbols=yes } fi ;; esac # Prepare the list of exported symbols if test -z "$export_symbols"; then if test yes = "$always_export_symbols" || test -n "$export_symbols_regex"; then func_verbose "generating symbol list for '$libname.la'" export_symbols=$output_objdir/$libname.exp $opt_dry_run || $RM $export_symbols cmds=$export_symbols_cmds save_ifs=$IFS; IFS='~' for cmd1 in $cmds; do IFS=$save_ifs # Take the normal branch if the nm_file_list_spec branch # doesn't work or if tool conversion is not needed. case $nm_file_list_spec~$to_tool_file_cmd in *~func_convert_file_noop | *~func_convert_file_msys_to_w32 | ~*) try_normal_branch=yes eval cmd=\"$cmd1\" func_len " $cmd" len=$func_len_result ;; *) try_normal_branch=no ;; esac if test yes = "$try_normal_branch" \ && { test "$len" -lt "$max_cmd_len" \ || test "$max_cmd_len" -le -1; } then func_show_eval "$cmd" 'exit $?' skipped_export=false elif test -n "$nm_file_list_spec"; then func_basename "$output" output_la=$func_basename_result save_libobjs=$libobjs save_output=$output output=$output_objdir/$output_la.nm func_to_tool_file "$output" libobjs=$nm_file_list_spec$func_to_tool_file_result func_append delfiles " $output" func_verbose "creating $NM input file list: $output" for obj in $save_libobjs; do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" done > "$output" eval cmd=\"$cmd1\" func_show_eval "$cmd" 'exit $?' output=$save_output libobjs=$save_libobjs skipped_export=false else # The command line is too long to execute in one step. func_verbose "using reloadable object file for export list..." skipped_export=: # Break out early, otherwise skipped_export may be # set to false by a later but shorter cmd. break fi done IFS=$save_ifs if test -n "$export_symbols_regex" && test : != "$skipped_export"; then func_show_eval '$EGREP -e "$export_symbols_regex" "$export_symbols" > "${export_symbols}T"' func_show_eval '$MV "${export_symbols}T" "$export_symbols"' fi fi fi if test -n "$export_symbols" && test -n "$include_expsyms"; then tmp_export_symbols=$export_symbols test -n "$orig_export_symbols" && tmp_export_symbols=$orig_export_symbols $opt_dry_run || eval '$ECHO "$include_expsyms" | $SP2NL >> "$tmp_export_symbols"' fi if test : != "$skipped_export" && test -n "$orig_export_symbols"; then # The given exports_symbols file has to be filtered, so filter it. func_verbose "filter symbol list for '$libname.la' to tag DATA exports" # FIXME: $output_objdir/$libname.filter potentially contains lots of # 's' commands, which not all seds can handle. GNU sed should be fine # though. Also, the filter scales superlinearly with the number of # global variables. join(1) would be nice here, but unfortunately # isn't a blessed tool. $opt_dry_run || $SED -e '/[ ,]DATA/!d;s,\(.*\)\([ \,].*\),s|^\1$|\1\2|,' < $export_symbols > $output_objdir/$libname.filter func_append delfiles " $export_symbols $output_objdir/$libname.filter" export_symbols=$output_objdir/$libname.def $opt_dry_run || $SED -f $output_objdir/$libname.filter < $orig_export_symbols > $export_symbols fi tmp_deplibs= for test_deplib in $deplibs; do case " $convenience " in *" $test_deplib "*) ;; *) func_append tmp_deplibs " $test_deplib" ;; esac done deplibs=$tmp_deplibs if test -n "$convenience"; then if test -n "$whole_archive_flag_spec" && test yes = "$compiler_needs_object" && test -z "$libobjs"; then # extract the archives, so we have objects to list. # TODO: could optimize this to just extract one archive. whole_archive_flag_spec= fi if test -n "$whole_archive_flag_spec"; then save_libobjs=$libobjs eval libobjs=\"\$libobjs $whole_archive_flag_spec\" test "X$libobjs" = "X " && libobjs= else gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $convenience func_append libobjs " $func_extract_archives_result" test "X$libobjs" = "X " && libobjs= fi fi if test yes = "$thread_safe" && test -n "$thread_safe_flag_spec"; then eval flag=\"$thread_safe_flag_spec\" func_append linker_flags " $flag" fi # Make a backup of the uninstalled library when relinking if test relink = "$opt_mode"; then $opt_dry_run || eval '(cd $output_objdir && $RM ${realname}U && $MV $realname ${realname}U)' || exit $? fi # Do each of the archive commands. if test yes = "$module" && test -n "$module_cmds"; then if test -n "$export_symbols" && test -n "$module_expsym_cmds"; then eval test_cmds=\"$module_expsym_cmds\" cmds=$module_expsym_cmds else eval test_cmds=\"$module_cmds\" cmds=$module_cmds fi else if test -n "$export_symbols" && test -n "$archive_expsym_cmds"; then eval test_cmds=\"$archive_expsym_cmds\" cmds=$archive_expsym_cmds else eval test_cmds=\"$archive_cmds\" cmds=$archive_cmds fi fi if test : != "$skipped_export" && func_len " $test_cmds" && len=$func_len_result && test "$len" -lt "$max_cmd_len" || test "$max_cmd_len" -le -1; then : else # The command line is too long to link in one step, link piecewise # or, if using GNU ld and skipped_export is not :, use a linker # script. # Save the value of $output and $libobjs because we want to # use them later. If we have whole_archive_flag_spec, we # want to use save_libobjs as it was before # whole_archive_flag_spec was expanded, because we can't # assume the linker understands whole_archive_flag_spec. # This may have to be revisited, in case too many # convenience libraries get linked in and end up exceeding # the spec. if test -z "$convenience" || test -z "$whole_archive_flag_spec"; then save_libobjs=$libobjs fi save_output=$output func_basename "$output" output_la=$func_basename_result # Clear the reloadable object creation command queue and # initialize k to one. test_cmds= concat_cmds= objlist= last_robj= k=1 if test -n "$save_libobjs" && test : != "$skipped_export" && test yes = "$with_gnu_ld"; then output=$output_objdir/$output_la.lnkscript func_verbose "creating GNU ld script: $output" echo 'INPUT (' > $output for obj in $save_libobjs do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" >> $output done echo ')' >> $output func_append delfiles " $output" func_to_tool_file "$output" output=$func_to_tool_file_result elif test -n "$save_libobjs" && test : != "$skipped_export" && test -n "$file_list_spec"; then output=$output_objdir/$output_la.lnk func_verbose "creating linker input file list: $output" : > $output set x $save_libobjs shift firstobj= if test yes = "$compiler_needs_object"; then firstobj="$1 " shift fi for obj do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" >> $output done func_append delfiles " $output" func_to_tool_file "$output" output=$firstobj\"$file_list_spec$func_to_tool_file_result\" else if test -n "$save_libobjs"; then func_verbose "creating reloadable object files..." output=$output_objdir/$output_la-$k.$objext eval test_cmds=\"$reload_cmds\" func_len " $test_cmds" len0=$func_len_result len=$len0 # Loop over the list of objects to be linked. for obj in $save_libobjs do func_len " $obj" func_arith $len + $func_len_result len=$func_arith_result if test -z "$objlist" || test "$len" -lt "$max_cmd_len"; then func_append objlist " $obj" else # The command $test_cmds is almost too long, add a # command to the queue. if test 1 -eq "$k"; then # The first file doesn't have a previous command to add. reload_objs=$objlist eval concat_cmds=\"$reload_cmds\" else # All subsequent reloadable object files will link in # the last one created. reload_objs="$objlist $last_robj" eval concat_cmds=\"\$concat_cmds~$reload_cmds~\$RM $last_robj\" fi last_robj=$output_objdir/$output_la-$k.$objext func_arith $k + 1 k=$func_arith_result output=$output_objdir/$output_la-$k.$objext objlist=" $obj" func_len " $last_robj" func_arith $len0 + $func_len_result len=$func_arith_result fi done # Handle the remaining objects by creating one last # reloadable object file. All subsequent reloadable object # files will link in the last one created. test -z "$concat_cmds" || concat_cmds=$concat_cmds~ reload_objs="$objlist $last_robj" eval concat_cmds=\"\$concat_cmds$reload_cmds\" if test -n "$last_robj"; then eval concat_cmds=\"\$concat_cmds~\$RM $last_robj\" fi func_append delfiles " $output" else output= fi ${skipped_export-false} && { func_verbose "generating symbol list for '$libname.la'" export_symbols=$output_objdir/$libname.exp $opt_dry_run || $RM $export_symbols libobjs=$output # Append the command to create the export file. test -z "$concat_cmds" || concat_cmds=$concat_cmds~ eval concat_cmds=\"\$concat_cmds$export_symbols_cmds\" if test -n "$last_robj"; then eval concat_cmds=\"\$concat_cmds~\$RM $last_robj\" fi } test -n "$save_libobjs" && func_verbose "creating a temporary reloadable object file: $output" # Loop through the commands generated above and execute them. save_ifs=$IFS; IFS='~' for cmd in $concat_cmds; do IFS=$save_ifs $opt_quiet || { func_quote_arg expand,pretty "$cmd" eval "func_echo $func_quote_arg_result" } $opt_dry_run || eval "$cmd" || { lt_exit=$? # Restore the uninstalled library and exit if test relink = "$opt_mode"; then ( cd "$output_objdir" && \ $RM "${realname}T" && \ $MV "${realname}U" "$realname" ) fi exit $lt_exit } done IFS=$save_ifs if test -n "$export_symbols_regex" && ${skipped_export-false}; then func_show_eval '$EGREP -e "$export_symbols_regex" "$export_symbols" > "${export_symbols}T"' func_show_eval '$MV "${export_symbols}T" "$export_symbols"' fi fi ${skipped_export-false} && { if test -n "$export_symbols" && test -n "$include_expsyms"; then tmp_export_symbols=$export_symbols test -n "$orig_export_symbols" && tmp_export_symbols=$orig_export_symbols $opt_dry_run || eval '$ECHO "$include_expsyms" | $SP2NL >> "$tmp_export_symbols"' fi if test -n "$orig_export_symbols"; then # The given exports_symbols file has to be filtered, so filter it. func_verbose "filter symbol list for '$libname.la' to tag DATA exports" # FIXME: $output_objdir/$libname.filter potentially contains lots of # 's' commands, which not all seds can handle. GNU sed should be fine # though. Also, the filter scales superlinearly with the number of # global variables. join(1) would be nice here, but unfortunately # isn't a blessed tool. $opt_dry_run || $SED -e '/[ ,]DATA/!d;s,\(.*\)\([ \,].*\),s|^\1$|\1\2|,' < $export_symbols > $output_objdir/$libname.filter func_append delfiles " $export_symbols $output_objdir/$libname.filter" export_symbols=$output_objdir/$libname.def $opt_dry_run || $SED -f $output_objdir/$libname.filter < $orig_export_symbols > $export_symbols fi } libobjs=$output # Restore the value of output. output=$save_output if test -n "$convenience" && test -n "$whole_archive_flag_spec"; then eval libobjs=\"\$libobjs $whole_archive_flag_spec\" test "X$libobjs" = "X " && libobjs= fi # Expand the library linking commands again to reset the # value of $libobjs for piecewise linking. # Do each of the archive commands. if test yes = "$module" && test -n "$module_cmds"; then if test -n "$export_symbols" && test -n "$module_expsym_cmds"; then cmds=$module_expsym_cmds else cmds=$module_cmds fi else if test -n "$export_symbols" && test -n "$archive_expsym_cmds"; then cmds=$archive_expsym_cmds else cmds=$archive_cmds fi fi fi if test -n "$delfiles"; then # Append the command to remove temporary files to $cmds. eval cmds=\"\$cmds~\$RM $delfiles\" fi # Add any objects from preloaded convenience libraries if test -n "$dlprefiles"; then gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $dlprefiles func_append libobjs " $func_extract_archives_result" test "X$libobjs" = "X " && libobjs= fi save_ifs=$IFS; IFS='~' for cmd in $cmds; do IFS=$sp$nl eval cmd=\"$cmd\" IFS=$save_ifs $opt_quiet || { func_quote_arg expand,pretty "$cmd" eval "func_echo $func_quote_arg_result" } $opt_dry_run || eval "$cmd" || { lt_exit=$? # Restore the uninstalled library and exit if test relink = "$opt_mode"; then ( cd "$output_objdir" && \ $RM "${realname}T" && \ $MV "${realname}U" "$realname" ) fi exit $lt_exit } done IFS=$save_ifs # Restore the uninstalled library and exit if test relink = "$opt_mode"; then $opt_dry_run || eval '(cd $output_objdir && $RM ${realname}T && $MV $realname ${realname}T && $MV ${realname}U $realname)' || exit $? if test -n "$convenience"; then if test -z "$whole_archive_flag_spec"; then func_show_eval '${RM}r "$gentop"' fi fi exit $EXIT_SUCCESS fi # Create links to the real library. for linkname in $linknames; do if test "$realname" != "$linkname"; then func_show_eval '(cd "$output_objdir" && $RM "$linkname" && $LN_S "$realname" "$linkname")' 'exit $?' fi done # If -module or -export-dynamic was specified, set the dlname. if test yes = "$module" || test yes = "$export_dynamic"; then # On all known operating systems, these are identical. dlname=$soname fi fi ;; obj) if test -n "$dlfiles$dlprefiles" || test no != "$dlself"; then func_warning "'-dlopen' is ignored for objects" fi case " $deplibs" in *\ -l* | *\ -L*) func_warning "'-l' and '-L' are ignored for objects" ;; esac test -n "$rpath" && \ func_warning "'-rpath' is ignored for objects" test -n "$xrpath" && \ func_warning "'-R' is ignored for objects" test -n "$vinfo" && \ func_warning "'-version-info' is ignored for objects" test -n "$release" && \ func_warning "'-release' is ignored for objects" case $output in *.lo) test -n "$objs$old_deplibs" && \ func_fatal_error "cannot build library object '$output' from non-libtool objects" libobj=$output func_lo2o "$libobj" obj=$func_lo2o_result ;; *) libobj= obj=$output ;; esac # Delete the old objects. $opt_dry_run || $RM $obj $libobj # Objects from convenience libraries. This assumes # single-version convenience libraries. Whenever we create # different ones for PIC/non-PIC, this we'll have to duplicate # the extraction. reload_conv_objs= gentop= # if reload_cmds runs $LD directly, get rid of -Wl from # whole_archive_flag_spec and hope we can get by with turning comma # into space. case $reload_cmds in *\$LD[\ \$]*) wl= ;; esac if test -n "$convenience"; then if test -n "$whole_archive_flag_spec"; then eval tmp_whole_archive_flags=\"$whole_archive_flag_spec\" test -n "$wl" || tmp_whole_archive_flags=`$ECHO "$tmp_whole_archive_flags" | $SED 's|,| |g'` reload_conv_objs=$reload_objs\ $tmp_whole_archive_flags else gentop=$output_objdir/${obj}x func_append generated " $gentop" func_extract_archives $gentop $convenience reload_conv_objs="$reload_objs $func_extract_archives_result" fi fi # If we're not building shared, we need to use non_pic_objs test yes = "$build_libtool_libs" || libobjs=$non_pic_objects # Create the old-style object. reload_objs=$objs$old_deplibs' '`$ECHO "$libobjs" | $SP2NL | $SED "/\.$libext$/d; /\.lib$/d; $lo2o" | $NL2SP`' '$reload_conv_objs output=$obj func_execute_cmds "$reload_cmds" 'exit $?' # Exit if we aren't doing a library object file. if test -z "$libobj"; then if test -n "$gentop"; then func_show_eval '${RM}r "$gentop"' fi exit $EXIT_SUCCESS fi test yes = "$build_libtool_libs" || { if test -n "$gentop"; then func_show_eval '${RM}r "$gentop"' fi # Create an invalid libtool object if no PIC, so that we don't # accidentally link it into a program. # $show "echo timestamp > $libobj" # $opt_dry_run || eval "echo timestamp > $libobj" || exit $? exit $EXIT_SUCCESS } if test -n "$pic_flag" || test default != "$pic_mode"; then # Only do commands if we really have different PIC objects. reload_objs="$libobjs $reload_conv_objs" output=$libobj func_execute_cmds "$reload_cmds" 'exit $?' fi if test -n "$gentop"; then func_show_eval '${RM}r "$gentop"' fi exit $EXIT_SUCCESS ;; prog) case $host in *cygwin*) func_stripname '' '.exe' "$output" output=$func_stripname_result.exe;; esac test -n "$vinfo" && \ func_warning "'-version-info' is ignored for programs" test -n "$release" && \ func_warning "'-release' is ignored for programs" $preload \ && test unknown,unknown,unknown = "$dlopen_support,$dlopen_self,$dlopen_self_static" \ && func_warning "'LT_INIT([dlopen])' not used. Assuming no dlopen support." case $host in *-*-rhapsody* | *-*-darwin1.[012]) # On Rhapsody replace the C library is the System framework compile_deplibs=`$ECHO " $compile_deplibs" | $SED 's/ -lc / System.ltframework /'` finalize_deplibs=`$ECHO " $finalize_deplibs" | $SED 's/ -lc / System.ltframework /'` ;; esac case $host in *-*-darwin*) # Don't allow lazy linking, it breaks C++ global constructors # But is supposedly fixed on 10.4 or later (yay!). if test CXX = "$tagname"; then case ${MACOSX_DEPLOYMENT_TARGET-10.0} in 10.[0123]) func_append compile_command " $wl-bind_at_load" func_append finalize_command " $wl-bind_at_load" ;; esac fi # Time to change all our "foo.ltframework" stuff back to "-framework foo" compile_deplibs=`$ECHO " $compile_deplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` finalize_deplibs=`$ECHO " $finalize_deplibs" | $SED 's% \([^ $]*\).ltframework% -framework \1%g'` ;; esac # move library search paths that coincide with paths to not yet # installed libraries to the beginning of the library search list new_libs= for path in $notinst_path; do case " $new_libs " in *" -L$path/$objdir "*) ;; *) case " $compile_deplibs " in *" -L$path/$objdir "*) func_append new_libs " -L$path/$objdir" ;; esac ;; esac done for deplib in $compile_deplibs; do case $deplib in -L*) case " $new_libs " in *" $deplib "*) ;; *) func_append new_libs " $deplib" ;; esac ;; *) func_append new_libs " $deplib" ;; esac done compile_deplibs=$new_libs func_append compile_command " $compile_deplibs" func_append finalize_command " $finalize_deplibs" if test -n "$rpath$xrpath"; then # If the user specified any rpath flags, then add them. for libdir in $rpath $xrpath; do # This is the magic to use -rpath. case "$finalize_rpath " in *" $libdir "*) ;; *) func_append finalize_rpath " $libdir" ;; esac done fi # Now hardcode the library paths rpath= hardcode_libdirs= for libdir in $compile_rpath $finalize_rpath; do if test -n "$hardcode_libdir_flag_spec"; then if test -n "$hardcode_libdir_separator"; then if test -z "$hardcode_libdirs"; then hardcode_libdirs=$libdir else # Just accumulate the unique libdirs. case $hardcode_libdir_separator$hardcode_libdirs$hardcode_libdir_separator in *"$hardcode_libdir_separator$libdir$hardcode_libdir_separator"*) ;; *) func_append hardcode_libdirs "$hardcode_libdir_separator$libdir" ;; esac fi else eval flag=\"$hardcode_libdir_flag_spec\" func_append rpath " $flag" fi elif test -n "$runpath_var"; then case "$perm_rpath " in *" $libdir "*) ;; *) func_append perm_rpath " $libdir" ;; esac fi case $host in *-*-cygwin* | *-*-mingw* | *-*-pw32* | *-*-os2* | *-cegcc*) testbindir=`$ECHO "$libdir" | $SED -e 's*/lib$*/bin*'` case :$dllsearchpath: in *":$libdir:"*) ;; ::) dllsearchpath=$libdir;; *) func_append dllsearchpath ":$libdir";; esac case :$dllsearchpath: in *":$testbindir:"*) ;; ::) dllsearchpath=$testbindir;; *) func_append dllsearchpath ":$testbindir";; esac ;; esac done # Substitute the hardcoded libdirs into the rpath. if test -n "$hardcode_libdir_separator" && test -n "$hardcode_libdirs"; then libdir=$hardcode_libdirs eval rpath=\" $hardcode_libdir_flag_spec\" fi compile_rpath=$rpath rpath= hardcode_libdirs= for libdir in $finalize_rpath; do if test -n "$hardcode_libdir_flag_spec"; then if test -n "$hardcode_libdir_separator"; then if test -z "$hardcode_libdirs"; then hardcode_libdirs=$libdir else # Just accumulate the unique libdirs. case $hardcode_libdir_separator$hardcode_libdirs$hardcode_libdir_separator in *"$hardcode_libdir_separator$libdir$hardcode_libdir_separator"*) ;; *) func_append hardcode_libdirs "$hardcode_libdir_separator$libdir" ;; esac fi else eval flag=\"$hardcode_libdir_flag_spec\" func_append rpath " $flag" fi elif test -n "$runpath_var"; then case "$finalize_perm_rpath " in *" $libdir "*) ;; *) func_append finalize_perm_rpath " $libdir" ;; esac fi done # Substitute the hardcoded libdirs into the rpath. if test -n "$hardcode_libdir_separator" && test -n "$hardcode_libdirs"; then libdir=$hardcode_libdirs eval rpath=\" $hardcode_libdir_flag_spec\" fi finalize_rpath=$rpath if test -n "$libobjs" && test yes = "$build_old_libs"; then # Transform all the library objects into standard objects. compile_command=`$ECHO "$compile_command" | $SP2NL | $SED "$lo2o" | $NL2SP` finalize_command=`$ECHO "$finalize_command" | $SP2NL | $SED "$lo2o" | $NL2SP` fi func_generate_dlsyms "$outputname" "@PROGRAM@" false # template prelinking step if test -n "$prelink_cmds"; then func_execute_cmds "$prelink_cmds" 'exit $?' fi wrappers_required=: case $host in *cegcc* | *mingw32ce*) # Disable wrappers for cegcc and mingw32ce hosts, we are cross compiling anyway. wrappers_required=false ;; *cygwin* | *mingw* ) test yes = "$build_libtool_libs" || wrappers_required=false ;; *) if test no = "$need_relink" || test yes != "$build_libtool_libs"; then wrappers_required=false fi ;; esac $wrappers_required || { # Replace the output file specification. compile_command=`$ECHO "$compile_command" | $SED 's%@OUTPUT@%'"$output"'%g'` link_command=$compile_command$compile_rpath # We have no uninstalled library dependencies, so finalize right now. exit_status=0 func_show_eval "$link_command" 'exit_status=$?' if test -n "$postlink_cmds"; then func_to_tool_file "$output" postlink_cmds=`func_echo_all "$postlink_cmds" | $SED -e 's%@OUTPUT@%'"$output"'%g' -e 's%@TOOL_OUTPUT@%'"$func_to_tool_file_result"'%g'` func_execute_cmds "$postlink_cmds" 'exit $?' fi # Delete the generated files. if test -f "$output_objdir/${outputname}S.$objext"; then func_show_eval '$RM "$output_objdir/${outputname}S.$objext"' fi exit $exit_status } if test -n "$compile_shlibpath$finalize_shlibpath"; then compile_command="$shlibpath_var=\"$compile_shlibpath$finalize_shlibpath\$$shlibpath_var\" $compile_command" fi if test -n "$finalize_shlibpath"; then finalize_command="$shlibpath_var=\"$finalize_shlibpath\$$shlibpath_var\" $finalize_command" fi compile_var= finalize_var= if test -n "$runpath_var"; then if test -n "$perm_rpath"; then # We should set the runpath_var. rpath= for dir in $perm_rpath; do func_append rpath "$dir:" done compile_var="$runpath_var=\"$rpath\$$runpath_var\" " fi if test -n "$finalize_perm_rpath"; then # We should set the runpath_var. rpath= for dir in $finalize_perm_rpath; do func_append rpath "$dir:" done finalize_var="$runpath_var=\"$rpath\$$runpath_var\" " fi fi if test yes = "$no_install"; then # We don't need to create a wrapper script. link_command=$compile_var$compile_command$compile_rpath # Replace the output file specification. link_command=`$ECHO "$link_command" | $SED 's%@OUTPUT@%'"$output"'%g'` # Delete the old output file. $opt_dry_run || $RM $output # Link the executable and exit func_show_eval "$link_command" 'exit $?' if test -n "$postlink_cmds"; then func_to_tool_file "$output" postlink_cmds=`func_echo_all "$postlink_cmds" | $SED -e 's%@OUTPUT@%'"$output"'%g' -e 's%@TOOL_OUTPUT@%'"$func_to_tool_file_result"'%g'` func_execute_cmds "$postlink_cmds" 'exit $?' fi exit $EXIT_SUCCESS fi case $hardcode_action,$fast_install in relink,*) # Fast installation is not supported link_command=$compile_var$compile_command$compile_rpath relink_command=$finalize_var$finalize_command$finalize_rpath func_warning "this platform does not like uninstalled shared libraries" func_warning "'$output' will be relinked during installation" ;; *,yes) link_command=$finalize_var$compile_command$finalize_rpath relink_command=`$ECHO "$compile_var$compile_command$compile_rpath" | $SED 's%@OUTPUT@%\$progdir/\$file%g'` ;; *,no) link_command=$compile_var$compile_command$compile_rpath relink_command=$finalize_var$finalize_command$finalize_rpath ;; *,needless) link_command=$finalize_var$compile_command$finalize_rpath relink_command= ;; esac # Replace the output file specification. link_command=`$ECHO "$link_command" | $SED 's%@OUTPUT@%'"$output_objdir/$outputname"'%g'` # Delete the old output files. $opt_dry_run || $RM $output $output_objdir/$outputname $output_objdir/lt-$outputname func_show_eval "$link_command" 'exit $?' if test -n "$postlink_cmds"; then func_to_tool_file "$output_objdir/$outputname" postlink_cmds=`func_echo_all "$postlink_cmds" | $SED -e 's%@OUTPUT@%'"$output_objdir/$outputname"'%g' -e 's%@TOOL_OUTPUT@%'"$func_to_tool_file_result"'%g'` func_execute_cmds "$postlink_cmds" 'exit $?' fi # Now create the wrapper script. func_verbose "creating $output" # Quote the relink command for shipping. if test -n "$relink_command"; then # Preserve any variables that may affect compiler behavior for var in $variables_saved_for_relink; do if eval test -z \"\${$var+set}\"; then relink_command="{ test -z \"\${$var+set}\" || $lt_unset $var || { $var=; export $var; }; }; $relink_command" elif eval var_value=\$$var; test -z "$var_value"; then relink_command="$var=; export $var; $relink_command" else func_quote_arg pretty "$var_value" relink_command="$var=$func_quote_arg_result; export $var; $relink_command" fi done func_quote eval cd "`pwd`" func_quote_arg pretty,unquoted "($func_quote_result; $relink_command)" relink_command=$func_quote_arg_unquoted_result fi # Only actually do things if not in dry run mode. $opt_dry_run || { # win32 will think the script is a binary if it has # a .exe suffix, so we strip it off here. case $output in *.exe) func_stripname '' '.exe' "$output" output=$func_stripname_result ;; esac # test for cygwin because mv fails w/o .exe extensions case $host in *cygwin*) exeext=.exe func_stripname '' '.exe' "$outputname" outputname=$func_stripname_result ;; *) exeext= ;; esac case $host in *cygwin* | *mingw* ) func_dirname_and_basename "$output" "" "." output_name=$func_basename_result output_path=$func_dirname_result cwrappersource=$output_path/$objdir/lt-$output_name.c cwrapper=$output_path/$output_name.exe $RM $cwrappersource $cwrapper trap "$RM $cwrappersource $cwrapper; exit $EXIT_FAILURE" 1 2 15 func_emit_cwrapperexe_src > $cwrappersource # The wrapper executable is built using the $host compiler, # because it contains $host paths and files. If cross- # compiling, it, like the target executable, must be # executed on the $host or under an emulation environment. $opt_dry_run || { $LTCC $LTCFLAGS -o $cwrapper $cwrappersource $STRIP $cwrapper } # Now, create the wrapper script for func_source use: func_ltwrapper_scriptname $cwrapper $RM $func_ltwrapper_scriptname_result trap "$RM $func_ltwrapper_scriptname_result; exit $EXIT_FAILURE" 1 2 15 $opt_dry_run || { # note: this script will not be executed, so do not chmod. if test "x$build" = "x$host"; then $cwrapper --lt-dump-script > $func_ltwrapper_scriptname_result else func_emit_wrapper no > $func_ltwrapper_scriptname_result fi } ;; * ) $RM $output trap "$RM $output; exit $EXIT_FAILURE" 1 2 15 func_emit_wrapper no > $output chmod +x $output ;; esac } exit $EXIT_SUCCESS ;; esac # See if we need to build an old-fashioned archive. for oldlib in $oldlibs; do case $build_libtool_libs in convenience) oldobjs="$libobjs_save $symfileobj" addlibs=$convenience build_libtool_libs=no ;; module) oldobjs=$libobjs_save addlibs=$old_convenience build_libtool_libs=no ;; *) oldobjs="$old_deplibs $non_pic_objects" $preload && test -f "$symfileobj" \ && func_append oldobjs " $symfileobj" addlibs=$old_convenience ;; esac if test -n "$addlibs"; then gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $addlibs func_append oldobjs " $func_extract_archives_result" fi # Do each command in the archive commands. if test -n "$old_archive_from_new_cmds" && test yes = "$build_libtool_libs"; then cmds=$old_archive_from_new_cmds else # Add any objects from preloaded convenience libraries if test -n "$dlprefiles"; then gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_extract_archives $gentop $dlprefiles func_append oldobjs " $func_extract_archives_result" fi # POSIX demands no paths to be encoded in archives. We have # to avoid creating archives with duplicate basenames if we # might have to extract them afterwards, e.g., when creating a # static archive out of a convenience library, or when linking # the entirety of a libtool archive into another (currently # not supported by libtool). if (for obj in $oldobjs do func_basename "$obj" $ECHO "$func_basename_result" done | sort | sort -uc >/dev/null 2>&1); then : else echo "copying selected object files to avoid basename conflicts..." gentop=$output_objdir/${outputname}x func_append generated " $gentop" func_mkdir_p "$gentop" save_oldobjs=$oldobjs oldobjs= counter=1 for obj in $save_oldobjs do func_basename "$obj" objbase=$func_basename_result case " $oldobjs " in " ") oldobjs=$obj ;; *[\ /]"$objbase "*) while :; do # Make sure we don't pick an alternate name that also # overlaps. newobj=lt$counter-$objbase func_arith $counter + 1 counter=$func_arith_result case " $oldobjs " in *[\ /]"$newobj "*) ;; *) if test ! -f "$gentop/$newobj"; then break; fi ;; esac done func_show_eval "ln $obj $gentop/$newobj || cp $obj $gentop/$newobj" func_append oldobjs " $gentop/$newobj" ;; *) func_append oldobjs " $obj" ;; esac done fi func_to_tool_file "$oldlib" func_convert_file_msys_to_w32 tool_oldlib=$func_to_tool_file_result eval cmds=\"$old_archive_cmds\" func_len " $cmds" len=$func_len_result if test "$len" -lt "$max_cmd_len" || test "$max_cmd_len" -le -1; then cmds=$old_archive_cmds elif test -n "$archiver_list_spec"; then func_verbose "using command file archive linking..." for obj in $oldobjs do func_to_tool_file "$obj" $ECHO "$func_to_tool_file_result" done > $output_objdir/$libname.libcmd func_to_tool_file "$output_objdir/$libname.libcmd" oldobjs=" $archiver_list_spec$func_to_tool_file_result" cmds=$old_archive_cmds else # the command line is too long to link in one step, link in parts func_verbose "using piecewise archive linking..." save_RANLIB=$RANLIB RANLIB=: objlist= concat_cmds= save_oldobjs=$oldobjs oldobjs= # Is there a better way of finding the last object in the list? 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IN NO EVENT SHALL THE # X CONSORTIUM BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER LIABILITY, WHETHER IN # AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM, OUT OF OR IN CONNEC- # TION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE SOFTWARE. # # Except as contained in this notice, the name of the X Consortium shall not # be used in advertising or otherwise to promote the sale, use or other deal- # ings in this Software without prior written authorization from the X Consor- # tium. # # # FSF changes to this file are in the public domain. # # Calling this script install-sh is preferred over install.sh, to prevent # 'make' implicit rules from creating a file called install from it # when there is no Makefile. # # This script is compatible with the BSD install script, but was written # from scratch. tab=' ' nl=' ' IFS=" $tab$nl" # Set DOITPROG to "echo" to test this script. doit=${DOITPROG-} doit_exec=${doit:-exec} # Put in absolute file names if you don't have them in your path; # or use environment vars. chgrpprog=${CHGRPPROG-chgrp} chmodprog=${CHMODPROG-chmod} chownprog=${CHOWNPROG-chown} cmpprog=${CMPPROG-cmp} cpprog=${CPPROG-cp} mkdirprog=${MKDIRPROG-mkdir} mvprog=${MVPROG-mv} rmprog=${RMPROG-rm} stripprog=${STRIPPROG-strip} posix_mkdir= # Desired mode of installed file. mode=0755 chgrpcmd= chmodcmd=$chmodprog chowncmd= mvcmd=$mvprog rmcmd="$rmprog -f" stripcmd= src= dst= dir_arg= dst_arg= copy_on_change=false is_target_a_directory=possibly usage="\ Usage: $0 [OPTION]... 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See the GNU # General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program; if not, see <https://www.gnu.org/licenses/>. # # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that # program. This Exception is an additional permission under section 7 # of the GNU General Public License, version 3 ("GPLv3"). # Please send patches to <config-patches@gnu.org>. # # Configuration subroutine to validate and canonicalize a configuration type. # Supply the specified configuration type as an argument. # If it is invalid, we print an error message on stderr and exit with code 1. # Otherwise, we print the canonical config type on stdout and succeed. # You can get the latest version of this script from: # https://git.savannah.gnu.org/gitweb/?p=config.git;a=blob_plain;f=config.sub # This file is supposed to be the same for all GNU packages # and recognize all the CPU types, system types and aliases # that are meaningful with *any* GNU software. # Each package is responsible for reporting which valid configurations # it does not support. The user should be able to distinguish # a failure to support a valid configuration from a meaningless # configuration. # The goal of this file is to map all the various variations of a given # machine specification into a single specification in the form: # CPU_TYPE-MANUFACTURER-OPERATING_SYSTEM # or in some cases, the newer four-part form: # CPU_TYPE-MANUFACTURER-KERNEL-OPERATING_SYSTEM # It is wrong to echo any other type of specification. me=`echo "$0" | sed -e 's,.*/,,'` usage="\ Usage: $0 [OPTION] CPU-MFR-OPSYS or ALIAS Canonicalize a configuration name. Options: -h, --help print this help, then exit -t, --time-stamp print date of last modification, then exit -v, --version print version number, then exit Report bugs and patches to <config-patches@gnu.org>." version="\ GNU config.sub ($timestamp) Copyright 1992-2017 Free Software Foundation, Inc. This is free software; see the source for copying conditions. There is NO warranty; not even for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE." help=" Try \`$me --help' for more information." # Parse command line while test $# -gt 0 ; do case $1 in --time-stamp | --time* | -t ) echo "$timestamp" ; exit ;; --version | -v ) echo "$version" ; exit ;; --help | --h* | -h ) echo "$usage"; exit ;; -- ) # Stop option processing shift; break ;; - ) # Use stdin as input. break ;; -* ) echo "$me: invalid option $1$help" exit 1 ;; *local*) # First pass through any local machine types. echo $1 exit ;; * ) break ;; esac done case $# in 0) echo "$me: missing argument$help" >&2 exit 1;; 1) ;; *) echo "$me: too many arguments$help" >&2 exit 1;; esac # Separate what the user gave into CPU-COMPANY and OS or KERNEL-OS (if any). # Here we must recognize all the valid KERNEL-OS combinations. maybe_os=`echo $1 | sed 's/^\(.*\)-\([^-]*-[^-]*\)$/\2/'` case $maybe_os in nto-qnx* | linux-gnu* | linux-android* | linux-dietlibc | linux-newlib* | \ linux-musl* | linux-uclibc* | uclinux-uclibc* | uclinux-gnu* | kfreebsd*-gnu* | \ knetbsd*-gnu* | netbsd*-gnu* | netbsd*-eabi* | \ kopensolaris*-gnu* | cloudabi*-eabi* | \ storm-chaos* | os2-emx* | rtmk-nova*) os=-$maybe_os basic_machine=`echo $1 | sed 's/^\(.*\)-\([^-]*-[^-]*\)$/\1/'` ;; android-linux) os=-linux-android basic_machine=`echo $1 | sed 's/^\(.*\)-\([^-]*-[^-]*\)$/\1/'`-unknown ;; *) basic_machine=`echo $1 | sed 's/-[^-]*$//'` if [ $basic_machine != $1 ] then os=`echo $1 | sed 's/.*-/-/'` else os=; fi ;; esac ### Let's recognize common machines as not being operating systems so ### that things like config.sub decstation-3100 work. We also ### recognize some manufacturers as not being operating systems, so we ### can provide default operating systems below. case $os in -sun*os*) # Prevent following clause from handling this invalid input. ;; -dec* | -mips* | -sequent* | -encore* | -pc532* | -sgi* | -sony* | \ -att* | -7300* | -3300* | -delta* | -motorola* | -sun[234]* | \ -unicom* | -ibm* | -next | -hp | -isi* | -apollo | -altos* | \ -convergent* | -ncr* | -news | -32* | -3600* | -3100* | -hitachi* |\ -c[123]* | -convex* | -sun | -crds | -omron* | -dg | -ultra | -tti* | \ -harris | -dolphin | -highlevel | -gould | -cbm | -ns | -masscomp | \ -apple | -axis | -knuth | -cray | -microblaze*) os= basic_machine=$1 ;; -bluegene*) os=-cnk ;; -sim | -cisco | -oki | -wec | -winbond) os= basic_machine=$1 ;; -scout) ;; -wrs) os=-vxworks basic_machine=$1 ;; -chorusos*) os=-chorusos basic_machine=$1 ;; -chorusrdb) os=-chorusrdb basic_machine=$1 ;; -hiux*) os=-hiuxwe2 ;; -sco6) os=-sco5v6 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco5) os=-sco3.2v5 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco4) os=-sco3.2v4 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco3.2.[4-9]*) os=`echo $os | sed -e 's/sco3.2./sco3.2v/'` basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco3.2v[4-9]*) # Don't forget version if it is 3.2v4 or newer. basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco5v6*) # Don't forget version if it is 3.2v4 or newer. basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco*) os=-sco3.2v2 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -udk*) basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -isc) os=-isc2.2 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -clix*) basic_machine=clipper-intergraph ;; -isc*) basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -lynx*178) os=-lynxos178 ;; -lynx*5) os=-lynxos5 ;; -lynx*) os=-lynxos ;; -ptx*) basic_machine=`echo $1 | sed -e 's/86-.*/86-sequent/'` ;; -psos*) os=-psos ;; -mint | -mint[0-9]*) basic_machine=m68k-atari os=-mint ;; esac # Decode aliases for certain CPU-COMPANY combinations. case $basic_machine in # Recognize the basic CPU types without company name. # Some are omitted here because they have special meanings below. 1750a | 580 \ | a29k \ | aarch64 | aarch64_be \ | alpha | alphaev[4-8] | alphaev56 | alphaev6[78] | alphapca5[67] \ | alpha64 | alpha64ev[4-8] | alpha64ev56 | alpha64ev6[78] | alpha64pca5[67] \ | am33_2.0 \ | arc | arceb \ | arm | arm[bl]e | arme[lb] | armv[2-8] | armv[3-8][lb] | armv7[arm] \ | avr | avr32 \ | ba \ | be32 | be64 \ | bfin \ | c4x | c8051 | clipper \ | d10v | d30v | dlx | dsp16xx \ | e2k | epiphany \ | fido | fr30 | frv | ft32 \ | h8300 | h8500 | hppa | hppa1.[01] | hppa2.0 | hppa2.0[nw] | hppa64 \ | hexagon \ | i370 | i860 | i960 | ia16 | ia64 \ | ip2k | iq2000 \ | k1om \ | le32 | le64 \ | lm32 \ | m32c | m32r | m32rle | m68000 | m68k | m88k \ | maxq | mb | microblaze | microblazeel | mcore | mep | metag \ | mips | mipsbe | mipseb | mipsel | mipsle \ | mips16 \ | mips64 | mips64el \ | mips64octeon | mips64octeonel \ | mips64orion | mips64orionel \ | mips64r5900 | mips64r5900el \ | mips64vr | mips64vrel \ | mips64vr4100 | mips64vr4100el \ | mips64vr4300 | mips64vr4300el \ | mips64vr5000 | mips64vr5000el \ | mips64vr5900 | mips64vr5900el \ | mipsisa32 | mipsisa32el \ | mipsisa32r2 | mipsisa32r2el \ | mipsisa32r6 | mipsisa32r6el \ | mipsisa64 | mipsisa64el \ | mipsisa64r2 | mipsisa64r2el \ | mipsisa64r6 | mipsisa64r6el \ | mipsisa64sb1 | mipsisa64sb1el \ | mipsisa64sr71k | mipsisa64sr71kel \ | mipsr5900 | mipsr5900el \ | mipstx39 | mipstx39el \ | mn10200 | mn10300 \ | moxie \ | mt \ | msp430 \ | nds32 | nds32le | nds32be \ | nios | nios2 | nios2eb | nios2el \ | ns16k | ns32k \ | open8 | or1k | or1knd | or32 \ | pdp10 | pdp11 | pj | pjl \ | powerpc | powerpc64 | powerpc64le | powerpcle \ | pru \ | pyramid \ | riscv32 | riscv64 \ | rl78 | rx \ | score \ | sh | sh[1234] | sh[24]a | sh[24]aeb | sh[23]e | sh[234]eb | sheb | shbe | shle | sh[1234]le | sh3ele \ | sh64 | sh64le \ | sparc | sparc64 | sparc64b | sparc64v | sparc86x | sparclet | sparclite \ | sparcv8 | sparcv9 | sparcv9b | sparcv9v \ | spu \ | tahoe | tic4x | tic54x | tic55x | tic6x | tic80 | tron \ | ubicom32 \ | v850 | v850e | v850e1 | v850e2 | v850es | v850e2v3 \ | visium \ | wasm32 \ | x86 | xc16x | xstormy16 | xtensa \ | z8k | z80) basic_machine=$basic_machine-unknown ;; c54x) basic_machine=tic54x-unknown ;; c55x) basic_machine=tic55x-unknown ;; c6x) basic_machine=tic6x-unknown ;; leon|leon[3-9]) basic_machine=sparc-$basic_machine ;; m6811 | m68hc11 | m6812 | m68hc12 | m68hcs12x | nvptx | picochip) basic_machine=$basic_machine-unknown os=-none ;; m88110 | m680[12346]0 | m683?2 | m68360 | m5200 | v70 | w65 | z8k) ;; ms1) basic_machine=mt-unknown ;; strongarm | thumb | xscale) basic_machine=arm-unknown ;; xgate) basic_machine=$basic_machine-unknown os=-none ;; xscaleeb) basic_machine=armeb-unknown ;; xscaleel) basic_machine=armel-unknown ;; # We use `pc' rather than `unknown' # because (1) that's what they normally are, and # (2) the word "unknown" tends to confuse beginning users. i*86 | x86_64) basic_machine=$basic_machine-pc ;; # Object if more than one company name word. *-*-*) echo Invalid configuration \`$1\': machine \`$basic_machine\' not recognized 1>&2 exit 1 ;; # Recognize the basic CPU types with company name. 580-* \ | a29k-* \ | aarch64-* | aarch64_be-* \ | alpha-* | alphaev[4-8]-* | alphaev56-* | alphaev6[78]-* \ | alpha64-* | alpha64ev[4-8]-* | alpha64ev56-* | alpha64ev6[78]-* \ | alphapca5[67]-* | alpha64pca5[67]-* | arc-* | arceb-* \ | arm-* | armbe-* | armle-* | armeb-* | armv*-* \ | avr-* | avr32-* \ | ba-* \ | be32-* | be64-* \ | bfin-* | bs2000-* \ | c[123]* | c30-* | [cjt]90-* | c4x-* \ | c8051-* | clipper-* | craynv-* | cydra-* \ | d10v-* | d30v-* | dlx-* \ | e2k-* | elxsi-* \ | f30[01]-* | f700-* | fido-* | fr30-* | frv-* | fx80-* \ | h8300-* | h8500-* \ | hppa-* | hppa1.[01]-* | hppa2.0-* | hppa2.0[nw]-* | hppa64-* \ | hexagon-* \ | i*86-* | i860-* | i960-* | ia16-* | ia64-* \ | ip2k-* | iq2000-* \ | k1om-* \ | le32-* | le64-* \ | lm32-* \ | m32c-* | m32r-* | m32rle-* \ | m68000-* | m680[012346]0-* | m68360-* | m683?2-* | m68k-* \ | m88110-* | m88k-* | maxq-* | mcore-* | metag-* \ | microblaze-* | microblazeel-* \ | mips-* | mipsbe-* | mipseb-* | mipsel-* | mipsle-* \ | mips16-* \ | mips64-* | mips64el-* \ | mips64octeon-* | mips64octeonel-* \ | mips64orion-* | mips64orionel-* \ | mips64r5900-* | mips64r5900el-* \ | mips64vr-* | mips64vrel-* \ | mips64vr4100-* | mips64vr4100el-* \ | mips64vr4300-* | mips64vr4300el-* \ | mips64vr5000-* | mips64vr5000el-* \ | mips64vr5900-* | mips64vr5900el-* \ | mipsisa32-* | mipsisa32el-* \ | mipsisa32r2-* | mipsisa32r2el-* \ | mipsisa32r6-* | mipsisa32r6el-* \ | mipsisa64-* | mipsisa64el-* \ | mipsisa64r2-* | mipsisa64r2el-* \ | mipsisa64r6-* | mipsisa64r6el-* \ | mipsisa64sb1-* | mipsisa64sb1el-* \ | mipsisa64sr71k-* | mipsisa64sr71kel-* \ | mipsr5900-* | mipsr5900el-* \ | mipstx39-* | mipstx39el-* \ | mmix-* \ | mt-* \ | msp430-* \ | nds32-* | nds32le-* | nds32be-* \ | nios-* | nios2-* | nios2eb-* | nios2el-* \ | none-* | np1-* | ns16k-* | ns32k-* \ | open8-* \ | or1k*-* \ | orion-* \ | pdp10-* | pdp11-* | pj-* | pjl-* | pn-* | power-* \ | powerpc-* | powerpc64-* | powerpc64le-* | powerpcle-* \ | pru-* \ | pyramid-* \ | riscv32-* | riscv64-* \ | rl78-* | romp-* | rs6000-* | rx-* \ | sh-* | sh[1234]-* | sh[24]a-* | sh[24]aeb-* | sh[23]e-* | sh[34]eb-* | sheb-* | shbe-* \ | shle-* | sh[1234]le-* | sh3ele-* | sh64-* | sh64le-* \ | sparc-* | sparc64-* | sparc64b-* | sparc64v-* | sparc86x-* | sparclet-* \ | sparclite-* \ | sparcv8-* | sparcv9-* | sparcv9b-* | sparcv9v-* | sv1-* | sx*-* \ | tahoe-* \ | tic30-* | tic4x-* | tic54x-* | tic55x-* | tic6x-* | tic80-* \ | tile*-* \ | tron-* \ | ubicom32-* \ | v850-* | v850e-* | v850e1-* | v850es-* | v850e2-* | v850e2v3-* \ | vax-* \ | visium-* \ | wasm32-* \ | we32k-* \ | x86-* | x86_64-* | xc16x-* | xps100-* \ | xstormy16-* | xtensa*-* \ | ymp-* \ | z8k-* | z80-*) ;; # Recognize the basic CPU types without company name, with glob match. xtensa*) basic_machine=$basic_machine-unknown ;; # Recognize the various machine names and aliases which stand # for a CPU type and a company and sometimes even an OS. 386bsd) basic_machine=i386-unknown os=-bsd ;; 3b1 | 7300 | 7300-att | att-7300 | pc7300 | safari | unixpc) basic_machine=m68000-att ;; 3b*) basic_machine=we32k-att ;; a29khif) basic_machine=a29k-amd os=-udi ;; abacus) basic_machine=abacus-unknown ;; adobe68k) basic_machine=m68010-adobe os=-scout ;; alliant | fx80) basic_machine=fx80-alliant ;; altos | altos3068) basic_machine=m68k-altos ;; am29k) basic_machine=a29k-none os=-bsd ;; amd64) basic_machine=x86_64-pc ;; amd64-*) basic_machine=x86_64-`echo $basic_machine | sed 's/^[^-]*-//'` ;; amdahl) basic_machine=580-amdahl os=-sysv ;; amiga | amiga-*) basic_machine=m68k-unknown ;; amigaos | amigados) basic_machine=m68k-unknown os=-amigaos ;; amigaunix | amix) basic_machine=m68k-unknown os=-sysv4 ;; apollo68) basic_machine=m68k-apollo os=-sysv ;; apollo68bsd) basic_machine=m68k-apollo os=-bsd ;; aros) basic_machine=i386-pc os=-aros ;; asmjs) basic_machine=asmjs-unknown ;; aux) basic_machine=m68k-apple os=-aux ;; balance) basic_machine=ns32k-sequent os=-dynix ;; blackfin) basic_machine=bfin-unknown os=-linux ;; blackfin-*) basic_machine=bfin-`echo $basic_machine | sed 's/^[^-]*-//'` os=-linux ;; bluegene*) basic_machine=powerpc-ibm os=-cnk ;; c54x-*) basic_machine=tic54x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c55x-*) basic_machine=tic55x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c6x-*) basic_machine=tic6x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c90) basic_machine=c90-cray os=-unicos ;; cegcc) basic_machine=arm-unknown os=-cegcc ;; convex-c1) basic_machine=c1-convex os=-bsd ;; convex-c2) basic_machine=c2-convex os=-bsd ;; convex-c32) basic_machine=c32-convex os=-bsd ;; convex-c34) basic_machine=c34-convex os=-bsd ;; convex-c38) basic_machine=c38-convex os=-bsd ;; cray | j90) basic_machine=j90-cray os=-unicos ;; craynv) basic_machine=craynv-cray os=-unicosmp ;; cr16 | cr16-*) basic_machine=cr16-unknown os=-elf ;; crds | unos) basic_machine=m68k-crds ;; crisv32 | crisv32-* | etraxfs*) basic_machine=crisv32-axis ;; cris | cris-* | etrax*) basic_machine=cris-axis ;; crx) basic_machine=crx-unknown os=-elf ;; da30 | da30-*) basic_machine=m68k-da30 ;; decstation | decstation-3100 | pmax | pmax-* | pmin | dec3100 | decstatn) basic_machine=mips-dec ;; decsystem10* | dec10*) basic_machine=pdp10-dec os=-tops10 ;; decsystem20* | dec20*) basic_machine=pdp10-dec os=-tops20 ;; delta | 3300 | motorola-3300 | motorola-delta \ | 3300-motorola | delta-motorola) basic_machine=m68k-motorola ;; delta88) basic_machine=m88k-motorola os=-sysv3 ;; dicos) basic_machine=i686-pc os=-dicos ;; djgpp) basic_machine=i586-pc os=-msdosdjgpp ;; dpx20 | dpx20-*) basic_machine=rs6000-bull os=-bosx ;; dpx2*) basic_machine=m68k-bull os=-sysv3 ;; e500v[12]) basic_machine=powerpc-unknown os=$os"spe" ;; e500v[12]-*) basic_machine=powerpc-`echo $basic_machine | sed 's/^[^-]*-//'` os=$os"spe" ;; ebmon29k) basic_machine=a29k-amd os=-ebmon ;; elxsi) basic_machine=elxsi-elxsi os=-bsd ;; encore | umax | mmax) basic_machine=ns32k-encore ;; es1800 | OSE68k | ose68k | ose | OSE) basic_machine=m68k-ericsson os=-ose ;; fx2800) basic_machine=i860-alliant ;; genix) basic_machine=ns32k-ns ;; gmicro) basic_machine=tron-gmicro os=-sysv ;; go32) basic_machine=i386-pc os=-go32 ;; h3050r* | hiux*) basic_machine=hppa1.1-hitachi os=-hiuxwe2 ;; h8300hms) basic_machine=h8300-hitachi os=-hms ;; h8300xray) basic_machine=h8300-hitachi os=-xray ;; h8500hms) basic_machine=h8500-hitachi os=-hms ;; harris) basic_machine=m88k-harris os=-sysv3 ;; hp300-*) basic_machine=m68k-hp ;; hp300bsd) basic_machine=m68k-hp os=-bsd ;; hp300hpux) basic_machine=m68k-hp os=-hpux ;; hp3k9[0-9][0-9] | hp9[0-9][0-9]) basic_machine=hppa1.0-hp ;; hp9k2[0-9][0-9] | hp9k31[0-9]) basic_machine=m68000-hp ;; hp9k3[2-9][0-9]) basic_machine=m68k-hp ;; hp9k6[0-9][0-9] | hp6[0-9][0-9]) basic_machine=hppa1.0-hp ;; hp9k7[0-79][0-9] | hp7[0-79][0-9]) basic_machine=hppa1.1-hp ;; hp9k78[0-9] | hp78[0-9]) # FIXME: really hppa2.0-hp basic_machine=hppa1.1-hp ;; hp9k8[67]1 | hp8[67]1 | hp9k80[24] | hp80[24] | hp9k8[78]9 | hp8[78]9 | hp9k893 | hp893) # FIXME: really hppa2.0-hp basic_machine=hppa1.1-hp ;; hp9k8[0-9][13679] | hp8[0-9][13679]) basic_machine=hppa1.1-hp ;; hp9k8[0-9][0-9] | hp8[0-9][0-9]) basic_machine=hppa1.0-hp ;; hppa-next) os=-nextstep3 ;; hppaosf) basic_machine=hppa1.1-hp os=-osf ;; hppro) basic_machine=hppa1.1-hp os=-proelf ;; i370-ibm* | ibm*) basic_machine=i370-ibm ;; i*86v32) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-sysv32 ;; i*86v4*) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-sysv4 ;; i*86v) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-sysv ;; i*86sol2) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-solaris2 ;; i386mach) basic_machine=i386-mach os=-mach ;; i386-vsta | vsta) basic_machine=i386-unknown os=-vsta ;; iris | iris4d) basic_machine=mips-sgi case $os in -irix*) ;; *) os=-irix4 ;; esac ;; isi68 | isi) basic_machine=m68k-isi os=-sysv ;; 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ps2) basic_machine=i386-ibm ;; pw32) basic_machine=i586-unknown os=-pw32 ;; rdos | rdos64) basic_machine=x86_64-pc os=-rdos ;; rdos32) basic_machine=i386-pc os=-rdos ;; rom68k) basic_machine=m68k-rom68k os=-coff ;; rm[46]00) basic_machine=mips-siemens ;; rtpc | rtpc-*) basic_machine=romp-ibm ;; s390 | s390-*) basic_machine=s390-ibm ;; s390x | s390x-*) basic_machine=s390x-ibm ;; sa29200) basic_machine=a29k-amd os=-udi ;; sb1) basic_machine=mipsisa64sb1-unknown ;; sb1el) basic_machine=mipsisa64sb1el-unknown ;; sde) basic_machine=mipsisa32-sde os=-elf ;; sei) basic_machine=mips-sei os=-seiux ;; sequent) basic_machine=i386-sequent ;; sh) basic_machine=sh-hitachi os=-hms ;; sh5el) basic_machine=sh5le-unknown ;; sh64) basic_machine=sh64-unknown ;; sparclite-wrs | simso-wrs) basic_machine=sparclite-wrs os=-vxworks ;; sps7) basic_machine=m68k-bull os=-sysv2 ;; spur) basic_machine=spur-unknown ;; st2000) basic_machine=m68k-tandem ;; stratus) basic_machine=i860-stratus os=-sysv4 ;; strongarm-* | thumb-*) basic_machine=arm-`echo $basic_machine | sed 's/^[^-]*-//'` ;; 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Ake) contributed MIS and NILE. if test "`(/bin/universe) 2>/dev/null`" = att ; then echo pyramid-pyramid-sysv3 else echo pyramid-pyramid-bsd fi exit ;; NILE*:*:*:dcosx) echo pyramid-pyramid-svr4 exit ;; DRS?6000:unix:4.0:6*) echo sparc-icl-nx6 exit ;; DRS?6000:UNIX_SV:4.2*:7* | DRS?6000:isis:4.2*:7*) case `/usr/bin/uname -p` in sparc) echo sparc-icl-nx7; exit ;; esac ;; s390x:SunOS:*:*) echo ${UNAME_MACHINE}-ibm-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; sun4H:SunOS:5.*:*) echo sparc-hal-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; sun4*:SunOS:5.*:* | tadpole*:SunOS:5.*:*) echo sparc-sun-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; i86pc:AuroraUX:5.*:* | i86xen:AuroraUX:5.*:*) echo i386-pc-auroraux${UNAME_RELEASE} exit ;; i86pc:SunOS:5.*:* | i86xen:SunOS:5.*:*) eval $set_cc_for_build SUN_ARCH=i386 # If there is a compiler, see if it is configured for 64-bit objects. # Note that the Sun cc does not turn __LP64__ into 1 like gcc does. # This test works for both compilers. if [ "$CC_FOR_BUILD" != no_compiler_found ]; then if (echo '#ifdef __amd64'; echo IS_64BIT_ARCH; echo '#endif') | \ (CCOPTS="" $CC_FOR_BUILD -E - 2>/dev/null) | \ grep IS_64BIT_ARCH >/dev/null then SUN_ARCH=x86_64 fi fi echo ${SUN_ARCH}-pc-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; sun4*:SunOS:6*:*) # According to config.sub, this is the proper way to canonicalize # SunOS6. 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The system name ranges from "MiNT" over "FreeMiNT" # to the lowercase version "mint" (or "freemint"). Finally # the system name "TOS" denotes a system which is actually not # MiNT. But MiNT is downward compatible to TOS, so this should # be no problem. atarist[e]:*MiNT:*:* | atarist[e]:*mint:*:* | atarist[e]:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; atari*:*MiNT:*:* | atari*:*mint:*:* | atarist[e]:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; *falcon*:*MiNT:*:* | *falcon*:*mint:*:* | *falcon*:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; milan*:*MiNT:*:* | milan*:*mint:*:* | *milan*:*TOS:*:*) echo m68k-milan-mint${UNAME_RELEASE} exit ;; hades*:*MiNT:*:* | hades*:*mint:*:* | *hades*:*TOS:*:*) echo m68k-hades-mint${UNAME_RELEASE} exit ;; *:*MiNT:*:* | *:*mint:*:* | *:*TOS:*:*) echo m68k-unknown-mint${UNAME_RELEASE} exit ;; m68k:machten:*:*) echo m68k-apple-machten${UNAME_RELEASE} exit ;; powerpc:machten:*:*) echo powerpc-apple-machten${UNAME_RELEASE} exit ;; RISC*:Mach:*:*) echo mips-dec-mach_bsd4.3 exit ;; RISC*:ULTRIX:*:*) echo mips-dec-ultrix${UNAME_RELEASE} exit ;; VAX*:ULTRIX*:*:*) echo vax-dec-ultrix${UNAME_RELEASE} exit ;; 2020:CLIX:*:* | 2430:CLIX:*:*) echo clipper-intergraph-clix${UNAME_RELEASE} exit ;; mips:*:*:UMIPS | mips:*:*:RISCos) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #ifdef __cplusplus #include <stdio.h> /* for printf() prototype */ int main (int argc, char *argv[]) { #else int main (argc, argv) int argc; char *argv[]; { #endif #if defined (host_mips) && defined (MIPSEB) #if defined (SYSTYPE_SYSV) printf ("mips-mips-riscos%ssysv\\n", argv[1]); exit (0); #endif #if defined (SYSTYPE_SVR4) printf ("mips-mips-riscos%ssvr4\\n", argv[1]); exit (0); #endif #if defined (SYSTYPE_BSD43) || defined(SYSTYPE_BSD) printf ("mips-mips-riscos%sbsd\\n", argv[1]); exit (0); #endif #endif exit (-1); } EOF $CC_FOR_BUILD -o $dummy $dummy.c && dummyarg=`echo "${UNAME_RELEASE}" | sed -n 's/\([0-9]*\).*/\1/p'` && SYSTEM_NAME=`$dummy $dummyarg` && { echo "$SYSTEM_NAME"; exit; } echo mips-mips-riscos${UNAME_RELEASE} exit ;; Motorola:PowerMAX_OS:*:*) echo powerpc-motorola-powermax exit ;; Motorola:*:4.3:PL8-*) echo powerpc-harris-powermax exit ;; Night_Hawk:*:*:PowerMAX_OS | Synergy:PowerMAX_OS:*:*) echo powerpc-harris-powermax exit ;; Night_Hawk:Power_UNIX:*:*) echo powerpc-harris-powerunix exit ;; m88k:CX/UX:7*:*) echo m88k-harris-cxux7 exit ;; m88k:*:4*:R4*) echo m88k-motorola-sysv4 exit ;; m88k:*:3*:R3*) echo m88k-motorola-sysv3 exit ;; AViiON:dgux:*:*) # DG/UX returns AViiON for all architectures UNAME_PROCESSOR=`/usr/bin/uname -p` if [ $UNAME_PROCESSOR = mc88100 ] || [ $UNAME_PROCESSOR = mc88110 ] then if [ ${TARGET_BINARY_INTERFACE}x = m88kdguxelfx ] || \ [ ${TARGET_BINARY_INTERFACE}x = x ] then echo m88k-dg-dgux${UNAME_RELEASE} else echo m88k-dg-dguxbcs${UNAME_RELEASE} fi else echo i586-dg-dgux${UNAME_RELEASE} fi exit ;; M88*:DolphinOS:*:*) # DolphinOS (SVR3) echo m88k-dolphin-sysv3 exit ;; M88*:*:R3*:*) # Delta 88k system running SVR3 echo m88k-motorola-sysv3 exit ;; XD88*:*:*:*) # Tektronix XD88 system running UTekV (SVR3) echo m88k-tektronix-sysv3 exit ;; Tek43[0-9][0-9]:UTek:*:*) # Tektronix 4300 system running UTek (BSD) echo m68k-tektronix-bsd exit ;; *:IRIX*:*:*) echo mips-sgi-irix`echo ${UNAME_RELEASE}|sed -e 's/-/_/g'` exit ;; ????????:AIX?:[12].1:2) # AIX 2.2.1 or AIX 2.1.1 is RT/PC AIX. echo romp-ibm-aix # uname -m gives an 8 hex-code CPU id exit ;; # Note that: echo "'`uname -s`'" gives 'AIX ' i*86:AIX:*:*) echo i386-ibm-aix exit ;; ia64:AIX:*:*) if [ -x /usr/bin/oslevel ] ; then IBM_REV=`/usr/bin/oslevel` else IBM_REV=${UNAME_VERSION}.${UNAME_RELEASE} fi echo ${UNAME_MACHINE}-ibm-aix${IBM_REV} exit ;; *:AIX:2:3) if grep bos325 /usr/include/stdio.h >/dev/null 2>&1; then eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #include <sys/systemcfg.h> main() { if (!__power_pc()) exit(1); puts("powerpc-ibm-aix3.2.5"); exit(0); } EOF if $CC_FOR_BUILD -o $dummy $dummy.c && SYSTEM_NAME=`$dummy` then echo "$SYSTEM_NAME" else echo rs6000-ibm-aix3.2.5 fi elif grep bos324 /usr/include/stdio.h >/dev/null 2>&1; then echo rs6000-ibm-aix3.2.4 else echo rs6000-ibm-aix3.2 fi exit ;; *:AIX:*:[4567]) IBM_CPU_ID=`/usr/sbin/lsdev -C -c processor -S available | sed 1q | awk '{ print $1 }'` if /usr/sbin/lsattr -El ${IBM_CPU_ID} | grep ' POWER' >/dev/null 2>&1; then IBM_ARCH=rs6000 else IBM_ARCH=powerpc fi if [ -x /usr/bin/lslpp ] ; then IBM_REV=`/usr/bin/lslpp -Lqc bos.rte.libc | awk -F: '{ print $3 }' | sed s/[0-9]*$/0/` else IBM_REV=${UNAME_VERSION}.${UNAME_RELEASE} fi echo ${IBM_ARCH}-ibm-aix${IBM_REV} exit ;; *:AIX:*:*) echo rs6000-ibm-aix exit ;; ibmrt:4.4BSD:*|romp-ibm:4.4BSD:*) echo romp-ibm-bsd4.4 exit ;; ibmrt:*BSD:*|romp-ibm:BSD:*) # covers RT/PC BSD and echo romp-ibm-bsd${UNAME_RELEASE} # 4.3 with uname added to exit ;; # report: romp-ibm BSD 4.3 *:BOSX:*:*) echo rs6000-bull-bosx exit ;; DPX/2?00:B.O.S.:*:*) echo m68k-bull-sysv3 exit ;; 9000/[34]??:4.3bsd:1.*:*) echo m68k-hp-bsd exit ;; hp300:4.4BSD:*:* | 9000/[34]??:4.3bsd:2.*:*) echo m68k-hp-bsd4.4 exit ;; 9000/[34678]??:HP-UX:*:*) HPUX_REV=`echo ${UNAME_RELEASE}|sed -e 's/[^.]*.[0B]*//'` case "${UNAME_MACHINE}" in 9000/31?) HP_ARCH=m68000 ;; 9000/[34]??) HP_ARCH=m68k ;; 9000/[678][0-9][0-9]) if [ -x /usr/bin/getconf ]; then sc_cpu_version=`/usr/bin/getconf SC_CPU_VERSION 2>/dev/null` sc_kernel_bits=`/usr/bin/getconf SC_KERNEL_BITS 2>/dev/null` case "${sc_cpu_version}" in 523) HP_ARCH=hppa1.0 ;; # CPU_PA_RISC1_0 528) HP_ARCH=hppa1.1 ;; # CPU_PA_RISC1_1 532) # CPU_PA_RISC2_0 case "${sc_kernel_bits}" in 32) HP_ARCH=hppa2.0n ;; 64) HP_ARCH=hppa2.0w ;; '') HP_ARCH=hppa2.0 ;; # HP-UX 10.20 esac ;; esac fi if [ "${HP_ARCH}" = "" ]; then eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #define _HPUX_SOURCE #include <stdlib.h> #include <unistd.h> int main () { #if defined(_SC_KERNEL_BITS) long bits = sysconf(_SC_KERNEL_BITS); #endif long cpu = sysconf (_SC_CPU_VERSION); switch (cpu) { case CPU_PA_RISC1_0: puts ("hppa1.0"); break; case CPU_PA_RISC1_1: puts ("hppa1.1"); break; case CPU_PA_RISC2_0: #if defined(_SC_KERNEL_BITS) switch (bits) { case 64: puts ("hppa2.0w"); break; case 32: puts ("hppa2.0n"); break; default: puts ("hppa2.0"); break; } break; #else /* !defined(_SC_KERNEL_BITS) */ puts ("hppa2.0"); break; #endif default: puts ("hppa1.0"); break; } exit (0); } EOF (CCOPTS="" $CC_FOR_BUILD -o $dummy $dummy.c 2>/dev/null) && HP_ARCH=`$dummy` test -z "$HP_ARCH" && HP_ARCH=hppa fi ;; esac if [ ${HP_ARCH} = hppa2.0w ] then eval $set_cc_for_build # hppa2.0w-hp-hpux* has a 64-bit kernel and a compiler generating # 32-bit code. hppa64-hp-hpux* has the same kernel and a compiler # generating 64-bit code. GNU and HP use different nomenclature: # # $ CC_FOR_BUILD=cc ./config.guess # => hppa2.0w-hp-hpux11.23 # $ CC_FOR_BUILD="cc +DA2.0w" ./config.guess # => hppa64-hp-hpux11.23 if echo __LP64__ | (CCOPTS="" $CC_FOR_BUILD -E - 2>/dev/null) | grep -q __LP64__ then HP_ARCH=hppa2.0w else HP_ARCH=hppa64 fi fi echo ${HP_ARCH}-hp-hpux${HPUX_REV} exit ;; ia64:HP-UX:*:*) HPUX_REV=`echo ${UNAME_RELEASE}|sed -e 's/[^.]*.[0B]*//'` echo ia64-hp-hpux${HPUX_REV} exit ;; 3050*:HI-UX:*:*) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #include <unistd.h> int main () { long cpu = sysconf (_SC_CPU_VERSION); /* The order matters, because CPU_IS_HP_MC68K erroneously returns true for CPU_PA_RISC1_0. CPU_IS_PA_RISC returns correct results, however. */ if (CPU_IS_PA_RISC (cpu)) { switch (cpu) { case CPU_PA_RISC1_0: puts ("hppa1.0-hitachi-hiuxwe2"); break; case CPU_PA_RISC1_1: puts ("hppa1.1-hitachi-hiuxwe2"); break; case CPU_PA_RISC2_0: puts ("hppa2.0-hitachi-hiuxwe2"); break; default: puts ("hppa-hitachi-hiuxwe2"); break; } } else if (CPU_IS_HP_MC68K (cpu)) puts ("m68k-hitachi-hiuxwe2"); else puts ("unknown-hitachi-hiuxwe2"); exit (0); } EOF $CC_FOR_BUILD -o $dummy $dummy.c && SYSTEM_NAME=`$dummy` && { echo "$SYSTEM_NAME"; exit; } echo unknown-hitachi-hiuxwe2 exit ;; 9000/7??:4.3bsd:*:* | 9000/8?[79]:4.3bsd:*:*) echo hppa1.1-hp-bsd exit ;; 9000/8??:4.3bsd:*:*) echo hppa1.0-hp-bsd exit ;; *9??*:MPE/iX:*:* | *3000*:MPE/iX:*:*) echo hppa1.0-hp-mpeix exit ;; hp7??:OSF1:*:* | hp8?[79]:OSF1:*:*) echo hppa1.1-hp-osf exit ;; hp8??:OSF1:*:*) echo hppa1.0-hp-osf exit ;; i*86:OSF1:*:*) if [ -x /usr/sbin/sysversion ] ; then echo ${UNAME_MACHINE}-unknown-osf1mk else echo ${UNAME_MACHINE}-unknown-osf1 fi exit ;; parisc*:Lites*:*:*) echo hppa1.1-hp-lites exit ;; C1*:ConvexOS:*:* | convex:ConvexOS:C1*:*) echo c1-convex-bsd exit ;; C2*:ConvexOS:*:* | convex:ConvexOS:C2*:*) if getsysinfo -f scalar_acc then echo c32-convex-bsd else echo c2-convex-bsd fi exit ;; C34*:ConvexOS:*:* | convex:ConvexOS:C34*:*) echo c34-convex-bsd exit ;; C38*:ConvexOS:*:* | convex:ConvexOS:C38*:*) echo c38-convex-bsd exit ;; C4*:ConvexOS:*:* | convex:ConvexOS:C4*:*) echo c4-convex-bsd exit ;; CRAY*Y-MP:*:*:*) echo ymp-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*[A-Z]90:*:*:*) echo ${UNAME_MACHINE}-cray-unicos${UNAME_RELEASE} \ | sed -e 's/CRAY.*\([A-Z]90\)/\1/' \ -e y/ABCDEFGHIJKLMNOPQRSTUVWXYZ/abcdefghijklmnopqrstuvwxyz/ \ -e 's/\.[^.]*$/.X/' exit ;; CRAY*TS:*:*:*) echo t90-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*T3E:*:*:*) echo alphaev5-cray-unicosmk${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*SV1:*:*:*) echo sv1-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; *:UNICOS/mp:*:*) echo craynv-cray-unicosmp${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; F30[01]:UNIX_System_V:*:* | F700:UNIX_System_V:*:*) FUJITSU_PROC=`uname -m | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz` FUJITSU_SYS=`uname -p | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz | sed -e 's/\///'` FUJITSU_REL=`echo ${UNAME_RELEASE} | sed -e 's/ /_/'` echo "${FUJITSU_PROC}-fujitsu-${FUJITSU_SYS}${FUJITSU_REL}" exit ;; 5000:UNIX_System_V:4.*:*) FUJITSU_SYS=`uname -p | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz | sed -e 's/\///'` FUJITSU_REL=`echo ${UNAME_RELEASE} | tr ABCDEFGHIJKLMNOPQRSTUVWXYZ abcdefghijklmnopqrstuvwxyz | sed -e 's/ /_/'` echo "sparc-fujitsu-${FUJITSU_SYS}${FUJITSU_REL}" exit ;; i*86:BSD/386:*:* | i*86:BSD/OS:*:* | *:Ascend\ Embedded/OS:*:*) echo ${UNAME_MACHINE}-pc-bsdi${UNAME_RELEASE} exit ;; sparc*:BSD/OS:*:*) echo sparc-unknown-bsdi${UNAME_RELEASE} exit ;; *:BSD/OS:*:*) echo ${UNAME_MACHINE}-unknown-bsdi${UNAME_RELEASE} exit ;; 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avr32*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; cris:Linux:*:*) echo ${UNAME_MACHINE}-axis-linux-${LIBC} exit ;; crisv32:Linux:*:*) echo ${UNAME_MACHINE}-axis-linux-${LIBC} exit ;; e2k:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; frv:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; hexagon:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; i*86:Linux:*:*) echo ${UNAME_MACHINE}-pc-linux-${LIBC} exit ;; ia64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; k1om:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; m32r*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; m68*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; mips:Linux:*:* | mips64:Linux:*:*) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #undef CPU #undef ${UNAME_MACHINE} #undef ${UNAME_MACHINE}el #if defined(__MIPSEL__) || defined(__MIPSEL) || defined(_MIPSEL) || defined(MIPSEL) CPU=${UNAME_MACHINE}el #else #if defined(__MIPSEB__) || defined(__MIPSEB) || defined(_MIPSEB) || defined(MIPSEB) CPU=${UNAME_MACHINE} #else CPU= #endif #endif EOF eval `$CC_FOR_BUILD -E $dummy.c 2>/dev/null | grep '^CPU'` test x"${CPU}" != x && { echo "${CPU}-unknown-linux-${LIBC}"; exit; } ;; mips64el:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; openrisc*:Linux:*:*) echo or1k-unknown-linux-${LIBC} exit ;; or32:Linux:*:* | or1k*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; padre:Linux:*:*) echo sparc-unknown-linux-${LIBC} exit ;; parisc64:Linux:*:* | hppa64:Linux:*:*) echo hppa64-unknown-linux-${LIBC} exit ;; parisc:Linux:*:* | hppa:Linux:*:*) # Look for CPU level case `grep '^cpu[^a-z]*:' /proc/cpuinfo 2>/dev/null | cut -d' ' -f2` in PA7*) echo hppa1.1-unknown-linux-${LIBC} ;; PA8*) echo hppa2.0-unknown-linux-${LIBC} ;; *) echo hppa-unknown-linux-${LIBC} ;; esac exit ;; ppc64:Linux:*:*) echo powerpc64-unknown-linux-${LIBC} exit ;; ppc:Linux:*:*) echo powerpc-unknown-linux-${LIBC} exit ;; ppc64le:Linux:*:*) echo powerpc64le-unknown-linux-${LIBC} exit ;; ppcle:Linux:*:*) echo powerpcle-unknown-linux-${LIBC} exit ;; riscv32:Linux:*:* | riscv64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; s390:Linux:*:* | s390x:Linux:*:*) echo ${UNAME_MACHINE}-ibm-linux-${LIBC} exit ;; sh64*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; sh*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; sparc:Linux:*:* | sparc64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; tile*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; vax:Linux:*:*) echo ${UNAME_MACHINE}-dec-linux-${LIBC} exit ;; x86_64:Linux:*:*) echo ${UNAME_MACHINE}-pc-linux-${LIBC} exit ;; xtensa*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-${LIBC} exit ;; i*86:DYNIX/ptx:4*:*) # ptx 4.0 does uname -s correctly, with DYNIX/ptx in there. # earlier versions are messed up and put the nodename in both # sysname and nodename. echo i386-sequent-sysv4 exit ;; i*86:UNIX_SV:4.2MP:2.*) # Unixware is an offshoot of SVR4, but it has its own version # number series starting with 2... # I am not positive that other SVR4 systems won't match this, # I just have to hope. -- rms. # Use sysv4.2uw... so that sysv4* matches it. echo ${UNAME_MACHINE}-pc-sysv4.2uw${UNAME_VERSION} exit ;; i*86:OS/2:*:*) # If we were able to find `uname', then EMX Unix compatibility # is probably installed. echo ${UNAME_MACHINE}-pc-os2-emx exit ;; i*86:XTS-300:*:STOP) echo ${UNAME_MACHINE}-unknown-stop exit ;; i*86:atheos:*:*) echo ${UNAME_MACHINE}-unknown-atheos exit ;; i*86:syllable:*:*) echo ${UNAME_MACHINE}-pc-syllable exit ;; i*86:LynxOS:2.*:* | i*86:LynxOS:3.[01]*:* | i*86:LynxOS:4.[02]*:*) echo i386-unknown-lynxos${UNAME_RELEASE} exit ;; i*86:*DOS:*:*) echo ${UNAME_MACHINE}-pc-msdosdjgpp exit ;; i*86:*:4.*:*) UNAME_REL=`echo ${UNAME_RELEASE} | sed 's/\/MP$//'` if grep Novell /usr/include/link.h >/dev/null 2>/dev/null; then echo ${UNAME_MACHINE}-univel-sysv${UNAME_REL} else echo ${UNAME_MACHINE}-pc-sysv${UNAME_REL} fi exit ;; i*86:*:5:[678]*) # UnixWare 7.x, OpenUNIX and OpenServer 6. case `/bin/uname -X | grep "^Machine"` in *486*) UNAME_MACHINE=i486 ;; *Pentium) UNAME_MACHINE=i586 ;; *Pent*|*Celeron) UNAME_MACHINE=i686 ;; esac echo ${UNAME_MACHINE}-unknown-sysv${UNAME_RELEASE}${UNAME_SYSTEM}${UNAME_VERSION} exit ;; i*86:*:3.2:*) if test -f /usr/options/cb.name; then UNAME_REL=`sed -n 's/.*Version //p' </usr/options/cb.name` echo ${UNAME_MACHINE}-pc-isc$UNAME_REL elif /bin/uname -X 2>/dev/null >/dev/null ; then UNAME_REL=`(/bin/uname -X|grep Release|sed -e 's/.*= //')` (/bin/uname -X|grep i80486 >/dev/null) && UNAME_MACHINE=i486 (/bin/uname -X|grep '^Machine.*Pentium' >/dev/null) \ && UNAME_MACHINE=i586 (/bin/uname -X|grep '^Machine.*Pent *II' >/dev/null) \ && UNAME_MACHINE=i686 (/bin/uname -X|grep '^Machine.*Pentium Pro' >/dev/null) \ && UNAME_MACHINE=i686 echo ${UNAME_MACHINE}-pc-sco$UNAME_REL else echo ${UNAME_MACHINE}-pc-sysv32 fi exit ;; pc:*:*:*) # Left here for compatibility: # uname -m prints for DJGPP always 'pc', but it prints nothing about # the processor, so we play safe by assuming i586. # Note: whatever this is, it MUST be the same as what config.sub # prints for the "djgpp" host, or else GDB configure will decide that # this is a cross-build. echo i586-pc-msdosdjgpp exit ;; Intel:Mach:3*:*) echo i386-pc-mach3 exit ;; paragon:*:*:*) echo i860-intel-osf1 exit ;; i860:*:4.*:*) # i860-SVR4 if grep Stardent /usr/include/sys/uadmin.h >/dev/null 2>&1 ; then echo i860-stardent-sysv${UNAME_RELEASE} # Stardent Vistra i860-SVR4 else # Add other i860-SVR4 vendors below as they are discovered. echo i860-unknown-sysv${UNAME_RELEASE} # Unknown i860-SVR4 fi exit ;; mini*:CTIX:SYS*5:*) # "miniframe" echo m68010-convergent-sysv exit ;; mc68k:UNIX:SYSTEM5:3.51m) echo m68k-convergent-sysv exit ;; M680?0:D-NIX:5.3:*) echo m68k-diab-dnix exit ;; M68*:*:R3V[5678]*:*) test -r /sysV68 && { echo 'm68k-motorola-sysv'; exit; } ;; 3[345]??:*:4.0:3.0 | 3[34]??A:*:4.0:3.0 | 3[34]??,*:*:4.0:3.0 | 3[34]??/*:*:4.0:3.0 | 4400:*:4.0:3.0 | 4850:*:4.0:3.0 | SKA40:*:4.0:3.0 | SDS2:*:4.0:3.0 | SHG2:*:4.0:3.0 | S7501*:*:4.0:3.0) OS_REL='' test -r /etc/.relid \ && OS_REL=.`sed -n 's/[^ ]* [^ ]* \([0-9][0-9]\).*/\1/p' < /etc/.relid` /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep entium >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } ;; 3[34]??:*:4.0:* | 3[34]??,*:*:4.0:*) /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4; exit; } ;; NCR*:*:4.2:* | MPRAS*:*:4.2:*) OS_REL='.3' test -r /etc/.relid \ && OS_REL=.`sed -n 's/[^ ]* [^ ]* \([0-9][0-9]\).*/\1/p' < /etc/.relid` /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep entium >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep pteron >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } ;; m68*:LynxOS:2.*:* | m68*:LynxOS:3.0*:*) echo m68k-unknown-lynxos${UNAME_RELEASE} exit ;; mc68030:UNIX_System_V:4.*:*) echo m68k-atari-sysv4 exit ;; TSUNAMI:LynxOS:2.*:*) echo sparc-unknown-lynxos${UNAME_RELEASE} exit ;; rs6000:LynxOS:2.*:*) echo rs6000-unknown-lynxos${UNAME_RELEASE} exit ;; PowerPC:LynxOS:2.*:* | PowerPC:LynxOS:3.[01]*:* | PowerPC:LynxOS:4.[02]*:*) echo powerpc-unknown-lynxos${UNAME_RELEASE} exit ;; SM[BE]S:UNIX_SV:*:*) echo mips-dde-sysv${UNAME_RELEASE} exit ;; RM*:ReliantUNIX-*:*:*) echo mips-sni-sysv4 exit ;; RM*:SINIX-*:*:*) echo mips-sni-sysv4 exit ;; *:SINIX-*:*:*) if uname -p 2>/dev/null >/dev/null ; then UNAME_MACHINE=`(uname -p) 2>/dev/null` echo ${UNAME_MACHINE}-sni-sysv4 else echo ns32k-sni-sysv fi exit ;; PENTIUM:*:4.0*:*) # Unisys `ClearPath HMP IX 4000' SVR4/MP effort # says <Richard.M.Bartel@ccMail.Census.GOV> echo i586-unisys-sysv4 exit ;; *:UNIX_System_V:4*:FTX*) # From Gerald Hewes <hewes@openmarket.com>. # How about differentiating between stratus architectures? -djm echo hppa1.1-stratus-sysv4 exit ;; *:*:*:FTX*) # From seanf@swdc.stratus.com. echo i860-stratus-sysv4 exit ;; i*86:VOS:*:*) # From Paul.Green@stratus.com. echo ${UNAME_MACHINE}-stratus-vos exit ;; *:VOS:*:*) # From Paul.Green@stratus.com. echo hppa1.1-stratus-vos exit ;; mc68*:A/UX:*:*) echo m68k-apple-aux${UNAME_RELEASE} exit ;; news*:NEWS-OS:6*:*) echo mips-sony-newsos6 exit ;; R[34]000:*System_V*:*:* | R4000:UNIX_SYSV:*:* | R*000:UNIX_SV:*:*) if [ -d /usr/nec ]; then echo mips-nec-sysv${UNAME_RELEASE} else echo mips-unknown-sysv${UNAME_RELEASE} fi exit ;; BeBox:BeOS:*:*) # BeOS running on hardware made by Be, PPC only. echo powerpc-be-beos exit ;; BeMac:BeOS:*:*) # BeOS running on Mac or Mac clone, PPC only. echo powerpc-apple-beos exit ;; BePC:BeOS:*:*) # BeOS running on Intel PC compatible. echo i586-pc-beos exit ;; BePC:Haiku:*:*) # Haiku running on Intel PC compatible. echo i586-pc-haiku exit ;; x86_64:Haiku:*:*) echo x86_64-unknown-haiku exit ;; SX-4:SUPER-UX:*:*) echo sx4-nec-superux${UNAME_RELEASE} exit ;; SX-5:SUPER-UX:*:*) echo sx5-nec-superux${UNAME_RELEASE} exit ;; SX-6:SUPER-UX:*:*) echo sx6-nec-superux${UNAME_RELEASE} exit ;; SX-7:SUPER-UX:*:*) echo sx7-nec-superux${UNAME_RELEASE} exit ;; SX-8:SUPER-UX:*:*) echo sx8-nec-superux${UNAME_RELEASE} exit ;; SX-8R:SUPER-UX:*:*) echo sx8r-nec-superux${UNAME_RELEASE} exit ;; SX-ACE:SUPER-UX:*:*) echo sxace-nec-superux${UNAME_RELEASE} exit ;; Power*:Rhapsody:*:*) echo powerpc-apple-rhapsody${UNAME_RELEASE} exit ;; *:Rhapsody:*:*) echo ${UNAME_MACHINE}-apple-rhapsody${UNAME_RELEASE} exit ;; *:Darwin:*:*) UNAME_PROCESSOR=`uname -p` || UNAME_PROCESSOR=unknown eval $set_cc_for_build if test "$UNAME_PROCESSOR" = unknown ; then UNAME_PROCESSOR=powerpc fi if test `echo "$UNAME_RELEASE" | sed -e 's/\..*//'` -le 10 ; then if [ "$CC_FOR_BUILD" != no_compiler_found ]; then if (echo '#ifdef __LP64__'; echo IS_64BIT_ARCH; echo '#endif') | \ (CCOPTS="" $CC_FOR_BUILD -E - 2>/dev/null) | \ grep IS_64BIT_ARCH >/dev/null then case $UNAME_PROCESSOR in i386) UNAME_PROCESSOR=x86_64 ;; powerpc) UNAME_PROCESSOR=powerpc64 ;; esac fi # On 10.4-10.6 one might compile for PowerPC via gcc -arch ppc if (echo '#ifdef __POWERPC__'; echo IS_PPC; echo '#endif') | \ (CCOPTS="" $CC_FOR_BUILD -E - 2>/dev/null) | \ grep IS_PPC >/dev/null then UNAME_PROCESSOR=powerpc fi fi elif test "$UNAME_PROCESSOR" = i386 ; then # Avoid executing cc on OS X 10.9, as it ships with a stub # that puts up a graphical alert prompting to install # developer tools. Any system running Mac OS X 10.7 or # later (Darwin 11 and later) is required to have a 64-bit # processor. This is not true of the ARM version of Darwin # that Apple uses in portable devices. 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See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to <bug-automake@gnu.org> or send patches to # <automake-patches@gnu.org>. nl=' ' # We need space, tab and new line, in precisely that order. Quoting is # there to prevent tools from complaining about whitespace usage. IFS=" "" $nl" file_conv= # func_file_conv build_file lazy # Convert a $build file to $host form and store it in $file # Currently only supports Windows hosts. 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See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program. If not, see <http://www.gnu.org/licenses/>. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This file is maintained in Automake, please report # bugs to <bug-automake@gnu.org> or send patches to # <automake-patches@gnu.org>. # func_error message func_error () { echo "$me: $1" 1>&2 exit 1 } file_conv= # func_file_conv build_file # Convert a $build file to $host form and store it in $file # Currently only supports Windows hosts. func_file_conv () { file=$1 case $file in / | /[!/]*) # absolute file, and not a UNC file if test -z "$file_conv"; then # lazily determine how to convert abs files case `uname -s` in MINGW*) file_conv=mingw ;; CYGWIN*) file_conv=cygwin ;; *) file_conv=wine ;; esac fi case $file_conv in mingw) file=`cmd //C echo "$file " | sed -e 's/"\(.*\) " *$/\1/'` ;; cygwin) file=`cygpath -m "$file" || echo "$file"` ;; wine) file=`winepath -w "$file" || echo "$file"` ;; esac ;; esac } # func_at_file at_file operation archive # Iterate over all members in AT_FILE performing OPERATION on ARCHIVE # for each of them. # When interpreting the content of the @FILE, do NOT use func_file_conv, # since the user would need to supply preconverted file names to # binutils ar, at least for MinGW. func_at_file () { operation=$2 archive=$3 at_file_contents=`cat "$1"` eval set x "$at_file_contents" shift for member do $AR -NOLOGO $operation:"$member" "$archive" || exit $? done } case $1 in '') func_error "no command. 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Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef IMGTRANSFORM_H #define IMGTRANSFORM_H #include <gnuastro/threads.h> /* Limits to account for floating point errors: */ #define ABSOLUTEFLTERROR 1e-10 #define RELATIVEFLTERROR 1e-6 /* Internal structure. */ struct iwpparams { /* General input parameters: */ struct warpparams *p; /* Thread parameters. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* Barrier to keep threads waiting. */ }; /* Extenal functions. */ void warp(struct warpparams *p); #endif ����������gnuastro-0.5/bin/warp/ui.h��������������������������������������������������������������������������0000644�0001750�0001750�00000004014�13174462540�012455� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_WARPS = GAL_OPTIONS_GROUP_AFTER_COMMON, }; /* Available letters for short options: b d g i j l n u v w x y z A B E G H J L O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_KEEPWCS = 'k', UI_KEY_COVEREDFRAC = 'C', UI_KEY_ALIGN = 'a', UI_KEY_ROTATE = 'r', UI_KEY_SCALE = 's', UI_KEY_FLIP = 'f', UI_KEY_SHEAR = 'e', UI_KEY_TRANSLATE = 't', UI_KEY_PROJECT = 'p', UI_KEY_MATRIX = 'm', UI_KEY_CENTERONCORNER = 'c', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_HSTARTWCS = 1000, UI_KEY_HENDWCS, }; /* Functions */ void ui_read_check_inputs_setup(int argc, char *argv[], struct warpparams *p); void ui_free_report(struct warpparams *p, struct timeval *t1); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/warp/args.h������������������������������������������������������������������������0000644�0001750�0001750�00000012774�13202610317�012775� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { /* Input. */ { "hstartwcs", UI_KEY_HSTARTWCS, "INT", 0, "Header keyword number to start reading WCS.", GAL_OPTIONS_GROUP_INPUT, &p->hstartwcs, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "hendwcs", UI_KEY_HENDWCS, "INT", 0, "Header keyword number to end reading WCS.", GAL_OPTIONS_GROUP_INPUT, &p->hendwcs, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Output. */ { "keepwcs", UI_KEY_KEEPWCS, 0, 0, "Do not apply warp to input's WCS", GAL_OPTIONS_GROUP_OUTPUT, &p->keepwcs, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "coveredfrac", UI_KEY_COVEREDFRAC, "FLT", 0, "Acceptable fraction of output pixel covered.", GAL_OPTIONS_GROUP_OUTPUT, &p->coveredfrac, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Warps:", UI_GROUP_WARPS }, { "align", UI_KEY_ALIGN, 0, 0, "Align the image and celestial axes.", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "rotate", UI_KEY_ROTATE, "FLT", 0, "Rotate by the given angle in degrees.", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "scale", UI_KEY_SCALE, "FLT[,FLT]", 0, "Scale along the given axis(es).", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "flip", UI_KEY_FLIP, "INT[,INT]", 0, "Flip along the given axis(es).", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "shear", UI_KEY_SHEAR, "FLT[,FLT]", 0, "Shear along the given axis(es).", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "translate", UI_KEY_TRANSLATE, "FLT[,FLT]", 0, "Translate along the given axis(es).", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "project", UI_KEY_PROJECT, "FLT[,FLT]", 0, "Project along the given axis(es).", UI_GROUP_WARPS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "matrix", UI_KEY_MATRIX, "STR", 0, "Raw transformation matrix, highest priority.", UI_GROUP_WARPS, &p->matrix, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_modular_warps_ll }, { "centeroncorner", UI_KEY_CENTERONCORNER, 0, 0, "Center of coordinates on first pixel corner.", UI_GROUP_WARPS, &p->centeroncorner, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ����gnuastro-0.5/bin/warp/authors-cite.h����������������������������������������������������������������0000644�0001750�0001750�00000002756�13211076737�014463� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ������������������gnuastro-0.5/bin/warp/main.h������������������������������������������������������������������������0000644�0001750�0001750�00000005540�13125721536�012770� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "Warp" /* Program full name. */ #define PROGRAM_EXEC "astwarp" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Main program structure. */ struct warpparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ char *inputname; /* Name of input file. */ size_t hstartwcs; /* Header keyword No. to start reading WCS. */ size_t hendwcs; /* Header keyword No. to end reading WCS. */ uint8_t keepwcs; /* Wrap the warped/transfomed pixels. */ uint8_t centeroncorner; /* Shift center by 0.5 before and after. */ double coveredfrac; /* Acceptable fraction of output covered. */ /* Internal parameters: */ gal_data_t *input; /* Input data structure. */ gal_data_t *output; /* output data structure. */ gal_data_t *matrix; /* Warp/Transformation matrix. */ gal_data_t *modularll; /* List of modular warpings. */ double *inverse; /* Inverse of the input matrix. */ double *inwcsmatrix; /* Input WCS matrix. */ double *pixelscale; /* Pixel scale of input image. */ time_t rawtime; /* Starting time of the program. */ size_t extinds[4]; /* Indexs of the minimum and maximum values. */ size_t ordinds[4]; /* Indexs of anticlockwise vertices. */ double outfpixval[2]; /* Pixel value of first output pixel. */ double opixarea; /* Area of output pix in units of input pix. */ }; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/warp/warp.c������������������������������������������������������������������������0000644�0001750�0001750�00000044715�13151366335�013020� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <float.h> #include <stdlib.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/polygon.h> #include "main.h" #include "warp.h" /***************************************************************/ /************** MACROS ******************/ /***************************************************************/ /* Multiply a 2 element vector with a transformation matrix and put the result in the 2 element output array. It is assumed that the input is from a flat coordinate systemy. */ #define mappoint(V, T, O) \ { \ (O)[0]=( ( (T)[0]*(V)[0] + (T)[1]*(V)[1] + (T)[2] ) \ / ( (T)[6]*(V)[0] + (T)[7]*(V)[1] + (T)[8] ) ); \ (O)[1]=( ( (T)[3]*(V)[0] + (T)[4]*(V)[1] + (T)[5] ) \ / ( (T)[6]*(V)[0] + (T)[7]*(V)[1] + (T)[8] ) ); \ } \ /* A pixel's center is an integer value. This function will give the integer value that is nearest to a floating point number. Works for both positive and negative values and includes floating point errors. nearestint_halfhigher(0.5f) --> 1.0f */ #define nearestint_halfhigher(D) \ (ceil((D)) - (D) > 0.5f \ + GAL_POLYGON_ROUND_ERR ? ceil((D))-1.0f : ceil((D))) /* Similar to `nearestint_halflower' but: nearestint_halflower(0.5f) --> 0.0f; */ #define nearestint_halflower(D) \ (ceil((D)) - (D) > 0.5f - GAL_POLYGON_ROUND_ERR ? ceil((D))-1.0f : ceil((D))) #define ceilwitherr(D) \ ( fabs( nearbyint((D)) - (D) ) < GAL_POLYGON_ROUND_ERR \ ? nearbyint((D)) : nearbyint((D))+1 ) /***************************************************************/ /************** Processing function ******************/ /***************************************************************/ static void * warp_onthread(void *inparam) { struct iwpparams *iwp=(struct iwpparams*)inparam; struct warpparams *p=iwp->p; size_t *extinds=p->extinds, *ordinds=p->ordinds; long is0=p->input->dsize[0], is1=p->input->dsize[1]; double area, filledarea, *input=p->input->array, v=NAN; size_t i, j, ind, os1=p->output->dsize[1], numcrn, numinput; long x, y, xstart, xend, ystart, yend; /* Might be negative */ double ocrn[8], icrn_base[8], icrn[8], *output=p->output->array; double pcrn[8], *outfpixval=p->outfpixval, ccrn[GAL_POLYGON_MAX_CORNERS]; for(i=0; (ind=iwp->indexs[i])!=GAL_BLANK_SIZE_T; ++i) { /* Initialize the output pixel value: */ numinput=0; output[ind]=filledarea=0.0f; /* Set the corners of this output pixel. The ind/os1 and ind%os1 start from 0. Note that the outfpixval already contains the correction for the fact that the FITS standard considers the center of first pixel to be at (1.0f, 1.0f).*/ ocrn[0]=(double)(ind%os1)-0.5f+outfpixval[0]; ocrn[1]=(double)(ind/os1)-0.5f+outfpixval[1]; ocrn[2]=(double)(ind%os1)+0.5f+outfpixval[0]; ocrn[3]=(double)(ind/os1)-0.5f+outfpixval[1]; ocrn[4]=(double)(ind%os1)-0.5f+outfpixval[0]; ocrn[5]=(double)(ind/os1)+0.5f+outfpixval[1]; ocrn[6]=(double)(ind%os1)+0.5f+outfpixval[0]; ocrn[7]=(double)(ind/os1)+0.5f+outfpixval[1]; /* Transform the four corners of the output pixel to the input image coordinates. */ for(j=0;j<4;++j) mappoint(&ocrn[j*2], p->inverse, &icrn_base[j*2]); /* Using the known relationships between the vertice locations, put everything in the right place: */ xstart = nearestint_halfhigher( icrn_base[extinds[0]] ); xend = nearestint_halflower( icrn_base[extinds[1]] ) + 1; ystart = nearestint_halfhigher( icrn_base[extinds[2]] ); yend = nearestint_halflower( icrn_base[extinds[3]] ) + 1; icrn[0]=icrn_base[ordinds[0]*2]; icrn[1]=icrn_base[ordinds[0]*2+1]; icrn[2]=icrn_base[ordinds[1]*2]; icrn[3]=icrn_base[ordinds[1]*2+1]; icrn[4]=icrn_base[ordinds[2]*2]; icrn[5]=icrn_base[ordinds[2]*2+1]; icrn[6]=icrn_base[ordinds[3]*2]; icrn[7]=icrn_base[ordinds[3]*2+1]; /* For a check: if(ind==9999) { printf("\n\n\nind: %zu: (%zu, %zu):\n", ind, ind%os1+1, ind/os1+1); for(j=0;j<4;++j) printf("(%.3f, %.3f) --> (%.3f, %.3f)\n", ocrn[j*2], ocrn[j*2+1], icrn_base[j*2], icrn_base[j*2+1]); printf("------- Ordered -------\n"); for(j=0;j<4;++j) printf("(%.3f, %.3f)\n", icrn[j*2], icrn[j*2+1]); printf("------- Start and ending pixels -------\n"); printf("X: %ld -- %ld\n", xstart, xend); printf("Y: %ld -- %ld\n", ystart, yend); } */ /* Go over all the input pixels that are covered. Note that x and y are the centers of the pixel. */ for(y=ystart;y<yend;++y) { /* If the pixel isn't in the image (note that the pixel coordinates start from 1), contine to next. Note that the pixel polygon should be counter clockwise. */ if( y<1 || y>is0 ) continue; pcrn[1]=y-0.5f; pcrn[3]=y-0.5f; pcrn[5]=y+0.5f; pcrn[7]=y+0.5f; for(x=xstart;x<xend;++x) { if( x<1 || x>is1 ) continue; /* Read the value of the input pixel. */ v=input[(y-1)*is1+x-1]; pcrn[0]=x-0.5f; pcrn[2]=x+0.5f; pcrn[4]=x+0.5f; pcrn[6]=x-0.5f; /* Find the overlapping (clipped) polygon: */ gal_polygon_clip(icrn, 4, pcrn, 4, ccrn, &numcrn); area=gal_polygon_area(ccrn, numcrn); /* Add the fractional value of this pixel. If this output pixel covers a NaN pixel in the input grid, then calculate the area of this NaN pixel to account for it later. */ if( !isnan(v) ) { ++numinput; filledarea+=area; output[ind]+=v*area; } /* For a polygon check: if(ind==9999) { printf("%zu -- (%zd, %zd):\n", ind, x, y); printf("icrn:\n"); for(j=0;j<4;++j) printf("\t%.3f, %.3f\n", icrn[j*2], icrn[j*2+1]); printf("pcrn:\n"); for(j=0;j<4;++j) printf("\t%.3f, %.3f\n", pcrn[j*2], pcrn[j*2+1]); printf("ccrn:\n"); for(j=0;j<numcrn;++j) printf("\t%.3f, %.3f\n", ccrn[j*2], ccrn[j*2+1]); printf("[%zu]: %.3f of [%ld, %ld]: %f\n", ind, gal_polygon_area(ccrn, numcrn), x, y, input[(y-1)*is1+x-1]); } */ /* For a simple pixel value check: if(ind==97387) printf("%f --> (%zu) %f\n", v*gal_polygon_area(ccrn, numcrn), numinput, output[ind]); */ } } /* See if the pixel value should be set to NaN or not (because of not enough coverage). */ if(numinput && filledarea/p->opixarea < p->coveredfrac-1e-5) numinput=0; /* Write the final value to disk: */ if(numinput==0) output[ind]=NAN; } /* Wait until all other threads finish. */ if(p->cp.numthreads>1) pthread_barrier_wait(iwp->b); return NULL; } /***************************************************************/ /************** Preparations ******************/ /***************************************************************/ /* Do all the preparations. Make the output array. We transform the four corners of the image into the output space. To find the four sides of the image. About fpixel and lpixel. The point is that we don't want to spend time, transforming any pixels which we know will not be in the input image. Find the proper order of transformed pixel corners from the output array to the input array. The order is fixed for all the pixels in the image altough the scale might change. */ static void warp_preparations(struct warpparams *p) { double is0=p->input->dsize[0], is1=p->input->dsize[1]; double output[8], forarea[8]; double icrn[8]={0,0,0,0,0,0,0,0}; size_t i, *extinds=p->extinds, dsize[2]; double xmin=DBL_MAX, xmax=-DBL_MAX, ymin=DBL_MAX, ymax=-DBL_MAX; double ocrn[8]={0.5f,0.5f, 1.5f,0.5f, 0.5f,1.5f, 1.5f, 1.5f}; double input[8]={ 0.5f, 0.5f, is1+0.5f, 0.5f, 0.5f, is0+0.5f, is1+0.5f, is0+0.5f }; /* Find the range of pixels of the input image. All the input positions are moved to the negative by half a pixel since the center of the pixel is an integer value.*/ for(i=0;i<4;++i) { mappoint(&input[i*2], (double *)(p->matrix->array), &output[i*2]); if(output[i*2]<xmin) xmin = output[i*2]; if(output[i*2]>xmax) xmax = output[i*2]; if(output[i*2+1]<ymin) ymin = output[i*2+1]; if(output[i*2+1]>ymax) ymax = output[i*2+1]; } /* For a check: for(i=0;i<4;++i) printf("(%.3f, %.3f) --> (%.3f, %.3f)\n", input[i*2], input[i*2+1], output[i*2], output[i*2+1]); printf("xmin: %.3f\nxmax: %.3f\nymin: %.3f\nymax: %.3f\n", xmin, xmax, ymin, ymax); */ /* Set the final size of the image. The X axis is horizontal. The reason we are using the halflower variation of `nearestint' for the maximums is that these points are the farthest extremes of the input image. If they are half a pixel value, they should point to the pixel before. */ dsize[1]=nearestint_halflower(xmax)-nearestint_halfhigher(xmin)+1; dsize[0]=nearestint_halflower(ymax)-nearestint_halfhigher(ymin)+1; p->outfpixval[0]=nearestint_halfhigher(xmin); p->outfpixval[1]=nearestint_halfhigher(ymin); /* For a check: printf("Wrapped:\n"); printf("dsize [C]: (%zu, %zu)\n", dsize[0], dsize[1]); printf("outfpixval [FITS]: (%.4f, %.4f)\n", p->outfpixval[0], p->outfpixval[1]); */ /* We now know the size of the output and the starting and ending coordinates in the output image (bottom left corners of pixels) for the transformation. */ p->output=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 2, dsize, p->input->wcs, 0, p->cp.minmapsize, "Warped", p->input->unit, NULL); /* Order the corners of the inverse-transformed pixel (from the output to the input) in an anti-clockwise transformation. In a general homographic transform, the scales of the output pixels may change, but the relative positions of the corners will not. */ for(i=0;i<4;++i) { ocrn[i*2] += p->outfpixval[0]; ocrn[i*2+1] += p->outfpixval[1]; mappoint(&ocrn[i*2], p->inverse, &icrn[i*2]); } /* Order the transformed output pixel. */ gal_polygon_ordered_corners(icrn, 4, p->ordinds); /* Find the area of the output pixel in units of the input pixel, this is necessary if we are going to have NAN pixels in the image to account for the area lost due to a NAN value. */ for(i=0;i<4;++i) { forarea[2*i]=icrn[2*p->ordinds[i]]; forarea[2*i+1]=icrn[2*p->ordinds[i]+1]; } p->opixarea=gal_polygon_area(forarea, 4); /* Find which index after transformation will have the minimum and maximum positions along the two axises. We can't use the starting loop because that is based on the input image which can be not-a-square! So we do it here where pixels are squares. */ xmin=DBL_MAX; xmax=-DBL_MAX; ymin=DBL_MAX; ymax=-DBL_MAX; for(i=0;i<4;++i) { if(icrn[i*2]<xmin) { xmin=icrn[i*2]; extinds[0]=i*2; } if(icrn[i*2]>xmax) { xmax=icrn[i*2]; extinds[1]=i*2; } if(icrn[i*2+1]<ymin) { ymin=icrn[i*2+1]; extinds[2]=i*2+1; } if(icrn[i*2+1]>ymax) { ymax=icrn[i*2+1]; extinds[3]=i*2+1; } } /* For a check: for(i=0;i<4;++i) printf("(%.3f, %.3f) --> (%.3f, %.3f)\n", ocrn[i*2], ocrn[i*2+1], icrn[i*2], icrn[i*2+1]); printf("xmin: %.3f\nxmax: %.3f\nymin: %.3f\nymax: %.3f\n", xmin, xmax, ymin, ymax); */ } /* Correct the WCS coordinates (Multiply the 2x2 PC matrix of the WCS structure by the INVERSE of the transform in 2x2). Then Multiply the crpix array with the ACTUAL transformation matrix. */ void correct_wcs_save_output(struct warpparams *p) { size_t i; double tcrpix[3]; char keyword[9*FLEN_KEYWORD]; double *m=p->matrix->array, diff; struct wcsprm *wcs=p->output->wcs; gal_fits_list_key_t *headers=NULL; double *crpix=wcs->crpix, *w=p->inwcsmatrix; /* `tinv' is the 2 by 2 inverse matrix. Recall that `p->inverse' is 3 by 3 to account for homogeneous coordinates. */ double tinv[4]={p->inverse[0]/p->inverse[8], p->inverse[1]/p->inverse[8], p->inverse[3]/p->inverse[8], p->inverse[4]/p->inverse[8]}; /* Make the WCS corrections if necessary. */ if(p->keepwcs==0 && wcs) { /* Correct the input WCS matrix. Since we are re-writing the PC matrix from the full rotation matrix (including pixel scale), we'll also have to set the CDELT fields to 1. Just to be sure that the PC matrix is used in the end by WCSLIB, we'll also set altlin to 1.*/ wcs->altlin=1; wcs->cdelt[0] = wcs->cdelt[1] = 1.0f; wcs->pc[0] = w[0]*tinv[0] + w[1]*tinv[2]; wcs->pc[1] = w[0]*tinv[1] + w[1]*tinv[3]; wcs->pc[2] = w[2]*tinv[0] + w[3]*tinv[2]; wcs->pc[3] = w[2]*tinv[1] + w[3]*tinv[3]; /* Correct the CRPIX point. The +1 in the end of the last two lines is because FITS counts from 1. */ tcrpix[0] = m[0]*crpix[0]+m[1]*crpix[1]+m[2]; tcrpix[1] = m[3]*crpix[0]+m[4]*crpix[1]+m[5]; tcrpix[2] = m[6]*crpix[0]+m[7]*crpix[1]+m[8]; crpix[0] = tcrpix[0]/tcrpix[2] - p->outfpixval[0] + 1; crpix[1] = tcrpix[1]/tcrpix[2] - p->outfpixval[1] + 1; } /* Add the appropriate headers: */ gal_fits_key_write_filename("INF", p->inputname, &headers); for(i=0;i<9;++i) { sprintf(&keyword[i*FLEN_KEYWORD], "WMTX%zu_%zu", i/3+1, i%3+1); gal_fits_key_list_add_end(&headers, GAL_TYPE_FLOAT64, &keyword[i*FLEN_KEYWORD], 0, &m[i], 0, "Warp matrix element value", 0, NULL); } /* Due to floating point errors extremely small values of PC matrix can be set to zero and extremely small differences between PC1_1 and PC2_2 can be ignored. The reason for all the `fabs' functions is because the signs are usually different.*/ if( fabs(wcs->pc[1])<ABSOLUTEFLTERROR ) wcs->pc[1]=0.0f; if( fabs(wcs->pc[2])<ABSOLUTEFLTERROR ) wcs->pc[2]=0.0f; diff=fabs(wcs->pc[0])-fabs(wcs->pc[3]); if( fabs(diff/p->pixelscale[0])<RELATIVEFLTERROR ) wcs->pc[3] = ( (wcs->pc[3] < 0.0f ? -1.0f : 1.0f) * fabs(wcs->pc[0]) ); /* Save the output into the proper type and write it. */ if(p->cp.type!=p->output->type) p->output=gal_data_copy_to_new_type_free(p->output, p->cp.type); gal_fits_img_write(p->output, p->cp.output, headers, PROGRAM_NAME); } /***************************************************************/ /************** Outside function ******************/ /***************************************************************/ void warp(struct warpparams *p) { int err; pthread_t t; /* All thread ids saved in this, not used. */ pthread_attr_t attr; pthread_barrier_t b; struct iwpparams *iwp; size_t nt=p->cp.numthreads; size_t i, nb, *indexs, thrdcols; /* Array keeping thread parameters for each thread. */ errno=0; iwp=malloc(nt*sizeof *iwp); if(iwp==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for iwp", __func__, nt*sizeof *iwp); /* Prepare the output array and all the necessary things: */ warp_preparations(p); /* Distribute the output pixels into the threads: */ gal_threads_dist_in_threads(p->output->size, nt, &indexs, &thrdcols); /* Start the convolution. */ if(nt==1) { iwp[0].p=p; iwp[0].indexs=indexs; warp_onthread(&iwp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(p->output->size<nt) nb=p->output->size+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Spin off the threads: */ for(i=0;i<nt;++i) if(indexs[i*thrdcols]!=GAL_BLANK_SIZE_T) { iwp[i].p=p; iwp[i].b=&b; iwp[i].indexs=&indexs[i*thrdcols]; err=pthread_create(&t, &attr, warp_onthread, &iwp[i]); if(err) error(EXIT_FAILURE, 0, "%s: can't create thread %zu", __func__, i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } /* Save the output. */ correct_wcs_save_output(p); /* Free the allocated spaces: */ free(iwp); free(indexs); gal_data_free(p->output); } ���������������������������������������������������gnuastro-0.5/bin/warp/ui.c��������������������������������������������������������������������������0000644�0001750�0001750�00000070373�13216276304�012461� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro/threads.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will warp/transform the " "input image using an input coordinate matrix. Currently it accepts any " "general projective mapping (which includes affine mappings as a " "subset). \n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct warpparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_struct = p; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->poptions = program_options; cp->numthreads = gal_threads_number(); cp->coptions = gal_commonopts_options; /* Set the mandatory common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct warpparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->inputname) argp_error(state, "only one argument (input file) should be given"); else p->inputname=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /********** Modular matrix linked list *************/ /**************************************************************/ /* Save the codes of the user's desired modular warpings into the linked list. Because the types of these options are `GAL_TYPE_INVALID', this function will not be called when printing the full list of parameters and their values. */ static void * ui_add_to_modular_warps_ll(struct argp_option *option, char *arg, char *filename, size_t lineno, void *params) { size_t i; double tmp; gal_data_t *new; struct warpparams *p=(struct warpparams *)params; /* Parse the (possible) arguments. */ if(option->key==UI_KEY_ALIGN) { /* For functions the standard checking isn't done, so first, we'll make sure that if we are in a configuration file (where `arg!=NULL'), the value is either 0 or 1. */ if( arg && strcmp(arg, "0") && strcmp(arg, "1") ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the `--align' " "option takes no arguments. In a configuration file " "it can only have the values `1' or `0', indicating " "if it should be used or not"); /* Align doesn't take any values, but if called in a configuration file with a value of `0', we should ignore it. */ if(arg && *arg=='0') return NULL; /* Allocate the data structure. */ new=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 0, NULL, NULL, 0, -1, NULL, NULL, NULL); } else new=gal_options_parse_list_of_numbers(arg, filename, lineno); /* If this was a matrix, then put it in the matrix element of the main data structure. Otherwise, add the list of given values to the modular warpings list. */ if(option->key==UI_KEY_MATRIX) { /* Some sanity checks. */ if(p->matrix) error_at_line(EXIT_FAILURE, 0, filename, lineno, "only one matrix " "may be given, you can use multiple modular warpings"); if(new->size!=4 && new->size!=9) error_at_line(EXIT_FAILURE, 0, filename, lineno, "only a 4 or 9 " "element `matrix' is currently acceptable. `%s' has " "%zu elements", arg, new->size); /* Keep the matrix in the main structure. */ p->matrix=new; } else { /* No more than two numbers should be given for the modular warpings. */ if(new->size>2) error_at_line(EXIT_FAILURE, 0, filename, lineno, "%zu numbers " "given to the `%s' option. Modular warpings can " "accept 2 numbers at the most currently (for 2D " "datasets)", new->size, option->name); /* Some modular-warp specific sanity checks: rotate only needs one number, and flip's values should only be 0 and 1. */ if(option->key==UI_KEY_ROTATE) { if(new->size!=1) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the `rotate' " "option only takes one value (the angle of rotation). " "You have given: `%s'", arg); } else if (option->key==UI_KEY_FLIP) { for(i=0;i<new->size;++i) { tmp=((double *)(new->array))[i]; if(tmp!=0.0f && tmp!=1.0f) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`flip' " "only takes values of `1' and `0'. You have " "given `%s'", arg); } } /* Keep the final value. */ new->status=option->key; new->next=p->modularll; p->modularll=new; } return NULL; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ static void ui_check_options_and_arguments(struct warpparams *p) { /* Read the input.*/ if(p->inputname) { /* Make sure a HDU is given. */ if( gal_fits_name_is_fits(p->inputname) && p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified, you can use the `--hdu' " "(`-h') option and give it the HDU number (starting from " "zero), or extension name (generally, anything acceptable " "by CFITSIO)"); /* Read the input image as double type and its WCS structure. */ p->input=gal_fits_img_read_to_type(p->inputname, p->cp.hdu, GAL_TYPE_FLOAT64, p->cp.minmapsize, p->hstartwcs, p->hendwcs); if(p->input->wcs) { p->pixelscale=gal_wcs_pixel_scale(p->input->wcs); p->inwcsmatrix=gal_wcs_warp_matrix(p->input->wcs); } } else error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /*************** Matrix preparations ******************/ /**************************************************************/ static void ui_error_no_warps() { error(EXIT_FAILURE, 0, "no warping specified, you can either use the " "`--matrix' option for any low-level warp, or specify multipole " "modular warpings with options like `--rotate', `--scale' and etc. " "You can see the full list with the `--help' option"); } /* This function is mainly for easy checking/debugging. */ static void ui_matrix_print(double *matrix) { printf("%-10.3f%-10.3f%-10.3f\n", matrix[0], matrix[1], matrix[2]); printf("%-10.3f%-10.3f%-10.3f\n", matrix[3], matrix[4], matrix[5]); printf("%-10.3f%-10.3f%-10.3f\n", matrix[6], matrix[7], matrix[8]); } static void ui_matrix_prepare_raw(struct warpparams *p) { size_t *dsize; double *in=p->matrix->array, *final; /* If the matrix was 2D, then convert it to 3D. Note that we done a size check when reading the matrix, so at this point, it either has 9 elements, or 4. */ if(p->matrix->size==4) { /* Allocate the final matrix. */ final=gal_data_malloc_array(GAL_TYPE_FLOAT64, 9, __func__, "final"); /* Fill in the final 3x3 matrix from the 2x2 matrix. */ final[0]=in[0]; final[1]=in[1]; final[2]=0.0f; final[3]=in[2]; final[4]=in[3]; final[5]=0.0f; final[6]=0.0f; final[7]=0.0f; final[8]=1.0f; /* Free the old matrix array and put in the new one. */ free(p->matrix->array); p->matrix->size=9; p->matrix->array=final; } /* Correct the dimensional information, because the matrix was read as a single dimensional list of numbers. */ free(p->matrix->dsize); dsize=p->matrix->dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, 2, __func__, "dsize"); dsize[0]=dsize[1]=3; p->matrix->ndim=2; } /* Set the matrix so the image is aligned with the axises. Note that WCSLIB automatically fills the CRPI */ static void ui_matrix_make_align(struct warpparams *p, double *tmatrix) { double A, *w, *P, x[4]; /* Make sure the input image had a WCS structure. */ if(p->input->wcs==NULL) error(EXIT_FAILURE, 0, "%s (hdu: %s): no WCS information present, " "hence the `--align' option cannot be used", p->inputname, p->cp.hdu); /* Check if there is only two WCS axises: */ if(p->input->wcs->naxis!=2) error(EXIT_FAILURE, 0, "the WCS structure of %s (hdu: %s) has %d " "axises. For the `--align' option to operate it must be 2", p->inputname, p->cp.hdu, p->input->wcs->naxis); /* For help in reading, use aliases for the WCS matrix and pixel scale.*/ P=p->pixelscale; w=p->inwcsmatrix; /* Lets call the given WCS orientation `W', the rotation matrix we want to find as `X' and the final (aligned matrix) `P' (which is the pixel scale): x0 x1 w0 w1 -P0 0 x2 x3 * w2 w3 = 0 P1 Let's open up the matrix multiplication, so we can find the `X' elements as function of the `W' elements and `a'. x0*w0 + x1*w2 = -P0 (1) x0*w1 + x1*w3 = 0 (2) x2*w0 + x3*w2 = 0 (3) x2*w1 + x3*w3 = P1 (4) Let's bring the X with the smaller index in each equation to the left side: x0 = (-w2/w0)*x1 - P0/w0 (5) x0 = (-w3/w1)*x1 (6) x2 = (-w2/w0)*x3 (7) x2 = (-w3/w1)*x3 + P1/w1 (8) Using (5) and (6) we can find x0 and x1, by first eliminating x0: (-w2/w0)*x1 - P0/w0 = (-w3/w1)*x1 -> (w3/w1 - w2/w0) * x1 = P0/w0 For easy reading/writing, let's define: A = (w3/w1 - w2/w0) --> x1 = P0 / w0 / A --> x0 = -1 * x1 * w3 / w1 Similar to the above, we can find x2 and x3 from (7) and (8): (-w2/w0)*x3 = (-w3/w1)*x3 + P1/w1 -> (w3/w1 - w2/w0) * x3 = P1/w1 --> x3 = P1 / w1 / A --> x2 = -1 * x3 * w2 / w0 Note that when the image is already aligned (off-diagonals are zero), only the signs of the diagonal elements matter. */ if( w[1]==0.0f && w[2]==0.0f ) { x[0] = w[0]<0 ? 1.0f : -1.0f; /* Has to be negative. */ x[1] = 0.0f; x[2] = 0.0f; x[3] = w[3]>0 ? 1.0f : -1.0f; /* Has to be positive. */ } else { A = (w[3]/w[1]) - (w[2]/w[0]); x[1] = P[0] / w[0] / A; x[3] = P[1] / w[1] / A; x[0] = -1 * x[1] * w[3] / w[1]; x[2] = -1 * x[3] * w[2] / w[0]; } /* For a check: printf("ps: (%e, %e)\n", P[0], P[1]); printf("w:\n"); printf(" %.8e %.8e\n", w[0], w[1]); printf(" %.8e %.8e\n", w[2], w[3]); printf("x:\n"); printf(" %.8e %.8e\n", x[0], x[1]); printf(" %.8e %.8e\n", x[2], x[3]); exit(0); */ /* Put the matrix elements into the output array: */ tmatrix[0]=x[0]; tmatrix[1]=x[1]; tmatrix[2]=0.0f; tmatrix[3]=x[2]; tmatrix[4]=x[3]; tmatrix[5]=0.0f; tmatrix[6]=0.0f; tmatrix[7]=0.0f; tmatrix[8]=1.0f; } static void ui_matrix_inplacw_multiply(double *in, double *with) { /* `tin' will keep the values of the input array because we want to write the multiplication result in the input array. */ double tin[9]={in[0],in[1],in[2],in[3],in[4],in[5],in[6],in[7],in[8]}; /* For easy checking, here are the matrix/memory layouts: tin[0] tin[1] tin[2] with[0] with[1] with[2] tin[3] tin[4] tin[5] * with[3] with[4] with[5] tin[6] tin[7] tin[8] with[6] with[7] with[8] */ in[0] = tin[0]*with[0] + tin[1]*with[3] + tin[2]*with[6]; in[1] = tin[0]*with[1] + tin[1]*with[4] + tin[2]*with[7]; in[2] = tin[0]*with[2] + tin[1]*with[5] + tin[2]*with[8]; in[3] = tin[3]*with[0] + tin[4]*with[3] + tin[5]*with[6]; in[4] = tin[3]*with[1] + tin[4]*with[4] + tin[5]*with[7]; in[5] = tin[3]*with[2] + tin[4]*with[5] + tin[5]*with[8]; in[6] = tin[6]*with[0] + tin[7]*with[3] + tin[8]*with[6]; in[7] = tin[6]*with[1] + tin[7]*with[4] + tin[8]*with[7]; in[8] = tin[6]*with[2] + tin[7]*with[5] + tin[8]*with[8]; } static void ui_matrix_from_modular(struct warpparams *p) { gal_data_t *pop; size_t dsize[]={3,3}; double s, c, v1, v2, *final, module[9]={1,0,0, 0,1,0, 0,0,1}; /* Reverse the list of modular warpings to be in the same order as the user specified.*/ gal_list_data_reverse(&p->modularll); /* Allocate space for the final matrix. */ p->matrix=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 2, dsize, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); final=p->matrix->array; /* Fill in the final matrix to start with. */ final[0]=1.0f; final[1]=0.0f; final[2]=0.0f; final[3]=0.0f; final[4]=1.0f; final[5]=0.0f; final[6]=0.0f; final[7]=0.0f; final[8]=1.0f; /* Apply all modular warps. */ while(p->modularll) { /* Pop the top element. */ pop=gal_list_data_pop(&p->modularll); /* Set the (possibly) two values given for this warp. */ v1 = pop->ndim ? ((double *)(pop->array))[0] : 0.0f; v2 = pop->size>1 ? ((double *)(pop->array))[1] : v1; /* Depending on the type of the modular warp do it. Recall that the code for the warp, was stored in the `status' element of the data structure.*/ switch(pop->status) { case UI_KEY_ALIGN: ui_matrix_make_align(p, module); break; case UI_KEY_ROTATE: s = sin( v1 * M_PI / 180 ); c = cos( v1 * M_PI / 180 ); module[0]=c; module[1]=-1.0f*s; module[2]=0.0f; module[3]=s; module[4]=c; module[5]=0.0f; module[6]=0.0f; module[7]=0.0f; module[8]=1.0f; break; case UI_KEY_SCALE: module[0]=v1; module[1]=0.0f; module[2]=0.0f; module[3]=0.0f; module[4]=v2; module[5]=0.0f; module[6]=0.0f; module[7]=0.0f; module[8]=1.0f; break; case UI_KEY_FLIP: if ( v1==1.0f && v2==0.0f ) { module[0]=1.0f; module[1]=0.0f; module[3]=0.0f; module[4]=-1.0f; } else if ( v1==0.0f && v2==1.0f ) { module[0]=-1.0f; module[1]=0.0f; module[3]=0.0f; module[4]=1.0f; } else if ( v1==1.0f && v2==1.0f ) { module[0]=-1.0f; module[1]=0.0f; module[3]=0.0f; module[4]=-1.0f; } else /* When both are zero, just in case! */ { module[0]=1.0f; module[1]=0.0f; module[3]=0.0f; module[4]=1.0f; } module[2]=0.0f; module[5]=0.0f; module[6]=0.0f; module[7]=0.0f; module[8]=1.0f; break; case UI_KEY_SHEAR: module[0]=1.0f; module[1]=v1; module[2]=0.0f; module[3]=v2; module[4]=1.0f; module[5]=0.0f; module[6]=0.0f; module[7]=0.0f; module[8]=1.0f; break; case UI_KEY_TRANSLATE: module[0]=1.0f; module[1]=0.0f; module[2]=v1; module[3]=0.0f; module[4]=1.0f; module[5]=v2; module[6]=0.0f; module[7]=0.0f; module[8]=1.0f; break; case UI_KEY_PROJECT: module[0]=1.0f; module[1]=0.0f; module[2]=0.0f; module[3]=0.0f; module[4]=1.0f; module[5]=0.0f; module[6]=v1; module[7]=v2; module[8]=1.0f; break; default: error(EXIT_FAILURE, 0, "a bug! the code %d is not recognized as " "a valid modular warp in `ui_matrix_from_modular', this is " "not your fault, something in the programming has gone " "wrong. Please contact us at %s so we can correct it", pop->status, PACKAGE_BUGREPORT); } /* Multiply the main matrix with this modular matrix. */ ui_matrix_inplacw_multiply(p->matrix->array, module); /* Clean up. */ gal_data_free(pop); } } static void ui_matrix_center_on_corner(struct warpparams *p) { double *b, *d, *df; double before[9]={1,0,0.5,0,1,0.5,0,0,1}; double after[9]={1,0,-0.5,0,1,-0.5,0,0,1}; /* Shift the matrix by +0.5 so the coordinate center lies at the bottom left corner of the first pixel. Note that the updated values are written into the first argument of the function.*/ ui_matrix_inplacw_multiply(before, p->matrix->array); /* Translate them back into the proper FITS center. */ ui_matrix_inplacw_multiply(before, after); /* The final matrix is in `before', so put its values into the output matrix. */ b = before; df = (d=p->matrix->array) + p->matrix->size; do *d=*b++; while(++d<df); } static void ui_matrix_finalize(struct warpparams *p) { double *d, *df, *inv; /* If a matrix string is not given, the use the modular warpings. */ if(p->matrix) ui_matrix_prepare_raw(p); else if (p->modularll) ui_matrix_from_modular(p); else ui_error_no_warps(); /* If the user has asked for it, set the coordinate center on the corner of the first pixel. */ if(p->centeroncorner) ui_matrix_center_on_corner(p); /* Check if there are any non-normal numbers in the matrix: */ df=(d=p->matrix->array)+p->matrix->size; do if(!isfinite(*d++)) { ui_matrix_print(p->matrix->array); error(EXIT_FAILURE, 0, "%f is not a `normal' number in the " "input matrix shown above", *(d-1)); } while(d<df); /* Check if the determinant is not zero: */ d=p->matrix->array; if( d[0]*d[4]*d[8] + d[1]*d[5]*d[6] + d[2]*d[3]*d[7] - d[2]*d[4]*d[6] - d[1]*d[3]*d[8] - d[0]*d[5]*d[7] == 0 ) error(EXIT_FAILURE, 0, "the determinant of the given matrix " "is zero"); /* Note yet implemented: Check if the transformation is spatially invariant, in other words, if it differs between differet regions of the output. If it doesn't we can use this information for a more efficient processing. */ /* Make the inverse matrix: */ inv=p->inverse=gal_data_malloc_array(GAL_TYPE_FLOAT64, 9, __func__, "p->inverse"); inv[0] = d[4]*d[8] - d[5]*d[7]; inv[1] = d[2]*d[7] - d[1]*d[8]; inv[2] = d[1]*d[5] - d[2]*d[4]; inv[3] = d[5]*d[6] - d[3]*d[8]; inv[4] = d[0]*d[8] - d[2]*d[6]; inv[5] = d[2]*d[3] - d[0]*d[5]; inv[6] = d[3]*d[7] - d[4]*d[6]; inv[7] = d[1]*d[6] - d[0]*d[7]; inv[8] = d[0]*d[4] - d[1]*d[3]; /* Just for a test: { size_t i; printf("\nInput matrix:"); for(i=0;i<9;++i) { if(i%3==0) printf("\n"); printf("%-10.5f", d[i]); } printf("\n-----------\n"); printf("Inverse matrix:"); for(i=0;i<9;++i) { if(i%3==0) printf("\n"); printf("%-10.5f", inv[i]); } printf("\n\n"); } */ } /**************************************************************/ /************ General preparations ****************/ /**************************************************************/ /* When only one transformation is required, set the suffix for automatic output to more meaningful string. */ char * ui_set_suffix(struct warpparams *p) { /* A small independent sanity check: we either need a matrix or at least one modular warping. */ if(p->matrix==NULL && p->modularll==NULL) ui_error_no_warps(); /* We only want the more meaningful suffix when the list is defined AND when its only has one node (the `next' element is NULL). */ if(p->matrix==NULL && p->modularll->next==NULL) switch(p->modularll->status) { case UI_KEY_ALIGN: return "_aligned.fits"; case UI_KEY_ROTATE: return "_rotated.fits"; case UI_KEY_SCALE: return "_scaled.fits"; case UI_KEY_FLIP: return "_flipped.fits"; case UI_KEY_SHEAR: return "_sheared.fits"; case UI_KEY_TRANSLATE: return "_translated.fits"; case UI_KEY_PROJECT: return "_projected.fits"; default: error(EXIT_FAILURE, 0, "a bug! please contact us at %s so we can " "fix the problem. The modular warp code %d is not recognized " "in `ui_set_suffix'", PACKAGE_BUGREPORT, p->modularll->status); return NULL; } else return "_warped.fits"; } static void ui_preparations(struct warpparams *p) { /* Set the output name. This needs to be done before `ui_finalize_matrix' because that function will free the linked list of modular warpings which we will need to determine the suffix if no output name is specified. */ if(p->cp.output) gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); else p->cp.output=gal_checkset_automatic_output(&p->cp, p->inputname, ui_set_suffix(p)); /* Prepare the final warping matrix. */ ui_matrix_finalize(p); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct warpparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Everything is ready, notify the user of the program starting. */ if(!p->cp.quiet) { double *matrix=p->matrix->array; printf(PROGRAM_NAME" started on %s", ctime(&p->rawtime)); printf(" Using %zu CPU thread%s\n", p->cp.numthreads, p->cp.numthreads==1 ? "." : "s."); printf(" Input: %s (hdu: %s)\n", p->inputname, p->cp.hdu); printf(" matrix:" "\n\t%.4f %.4f %.4f" "\n\t%.4f %.4f %.4f" "\n\t%.4f %.4f %.4f\n", matrix[0], matrix[1], matrix[2], matrix[3], matrix[4], matrix[5], matrix[6], matrix[7], matrix[8]); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct warpparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->cp.hdu); free(p->cp.output); gal_data_free(p->input); gal_data_free(p->matrix); if(p->pixelscale) free(p->pixelscale); if(p->inwcsmatrix) free(p->inwcsmatrix); /* Report how long the operation took. */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/warp/main.c������������������������������������������������������������������������0000644�0001750�0001750�00000003005�13121462410�012742� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Warp - Warp images using projective mapping. Warp is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "warp.h" int main (int argc, char *argv[]) { struct timeval t1; struct warpparams p={{{0},0},0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run Warp */ warp(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/warp/Makefile.in�������������������������������������������������������������������0000644�0001750�0001750�00000211221�13217217706�013734� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; 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@GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BIND = @GNULIB_BIND@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME 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uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/warp/astwarp.conf������������������������������������������������������������������0000644�0001750�0001750�00000001721�13121462410�014205� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Warp. # Warp is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. 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This file is offered as-is, without any # warranty. # Input: # Output: coveredfrac 1.0 # Common parameters type float32 �����������������������������������������������gnuastro-0.5/bin/warp/Makefile.am�������������������������������������������������������������������0000644�0001750�0001750�00000002552�13121462410�013714� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astwarp astwarp_LDADD = -lgnuastro astwarp_SOURCES = main.c ui.c warp.c EXTRA_DIST = main.h authors-cite.h args.h ui.h warp.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astwarp.conf ������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/�����������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220467�012064� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/table.h����������������������������������������������������������������������0000644�0001750�0001750�00000002054�13121462410�013233� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef TABLE_H #define TABLE_H void table(struct tableparams *p); #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/ui.h�������������������������������������������������������������������������0000644�0001750�0001750�00000003044�13174462540�012575� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Available letters for short options: a b d e f g j k l m n p r s t u v w x y z A B C E G H J L O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_COLUMN = 'c', UI_KEY_INFORMATION = 'i', /* Only with long version (start with a value 1000, the rest will be set automatically). */ }; void ui_read_check_inputs_setup(int argc, char *argv[], struct tableparams *p); void ui_free_report(struct tableparams *p); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/args.h�����������������������������������������������������������������������0000644�0001750�0001750�00000004334�13121462410�013103� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { { "column", UI_KEY_COLUMN, "STR", 0, "Column number (counting from 1) or search string.", GAL_OPTIONS_GROUP_INPUT, &p->columns, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "information", UI_KEY_INFORMATION, 0, 0, "Only print table and column information.", GAL_OPTIONS_GROUP_OPERATING_MODE, &p->information, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/authors-cite.h���������������������������������������������������������������0000644�0001750�0001750�00000002767�13211076737�014603� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ���������gnuastro-0.5/bin/table/main.h�����������������������������������������������������������������������0000644�0001750�0001750�00000003726�13121462410�013077� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "Table" /* Program full name. */ #define PROGRAM_EXEC "asttable" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Main program parameters structure */ struct tableparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ char *filename; /* Input filename. */ gal_list_str_t *columns; /* List of given columns. */ uint8_t information; /* ==1, only print FITS information. */ /* Output: */ gal_data_t *table; /* Linked list of output table columns. */ gal_data_t *allcolinfo; /* Information of all the columns. */ time_t rawtime; /* Starting time of the program. */ }; #endif ������������������������������������������gnuastro-0.5/bin/table/table.c����������������������������������������������������������������������0000644�0001750�0001750�00000003134�13175442274�013245� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <stdlib.h> #include <unistd.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro-internal/checkset.h> #include "main.h" /**************************************************************/ /*************** Top function *******************/ /**************************************************************/ void table(struct tableparams *p) { gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); gal_table_write(p->table, NULL, p->cp.tableformat, p->cp.output, "TABLE"); } ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/ui.c�������������������������������������������������������������������������0000644�0001750�0001750�00000025525�13211616535�012575� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/tableintern.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" can be used to view the " "information, select columns, or convert tables. The inputs and outputs " "can be plain text (with white-space or comma as delimiters), FITS ascii, " "or FITS binary tables. The output columns can either be selected by " "number (counting from 1), name or using regular expressions. For regular " "expressions, enclose the value to the `--column' (`-c') option in " "slashes (`\\', as in `-c\\^mag\\'). To print the selected columns on the " "command-line, don't specify an output file.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct tableparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_MINMAPSIZE: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct tableparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->filename) argp_error(state, "only one argument (input file) should be given"); else p->filename=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct tableparams *p) { /* Check if the format of the output table is valid, given the type of the output. */ gal_tableintern_check_fits_format(p->cp.output, p->cp.tableformat); } static void ui_check_options_and_arguments(struct tableparams *p) { /* Make sure an input file name was given and if it was a FITS file, that a HDU is also given. */ if(p->filename) { if( gal_fits_name_is_fits(p->filename) && p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified. When the input is a FITS " "file, a HDU must also be specified, you can use the `--hdu' " "(`-h') option and give it the HDU number (starting from " "zero), extension name, or anything acceptable by CFITSIO"); } else error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void ui_print_info_exit(struct tableparams *p) { char *tmp; int tableformat; gal_data_t *allcols; size_t i, numcols, numrows; /* Read the table information for the number of columns and rows. */ allcols=gal_table_info(p->filename, p->cp.hdu, &numcols, &numrows, &tableformat); /* If there was no actual data in the file, then inform the user */ if(allcols==NULL) error(EXIT_FAILURE, 0, "%s: no usable data rows", p->filename); /* Print the file information. */ printf("--------\n"); tmp=gal_fits_name_save_as_string(p->filename, p->cp.hdu); printf("%s\n", tmp); free(tmp); /* Print each column's information. */ gal_table_print_info(allcols, numcols, numrows); /* Free the information from all the columns. */ for(i=0;i<numcols;++i) gal_data_free_contents(&allcols[i]); free(allcols); /* Free the allocated spaces and exit. Otherwise, add the number of columns to the list if the user wanted to print the columns (didn't just want their information. */ ui_free_report(p); exit(EXIT_SUCCESS); } void ui_preparations(struct tableparams *p) { struct gal_options_common_params *cp=&p->cp; /* If there were no columns specified or the user has asked for information on the columns, we want the full set of columns. */ if(p->information) ui_print_info_exit(p); /* Read in the table columns. */ p->table=gal_table_read(p->filename, cp->hdu, p->columns, cp->searchin, cp->ignorecase, cp->minmapsize, NULL); /* If there was no actual data in the file, then inform the user and abort. */ if(p->table==NULL) error(EXIT_FAILURE, 0, "%s: no usable data rows (non-commented and " "non-blank lines)", p->filename); /* Now that the data columns are ready, we can free the string linked list. */ gal_list_str_free(p->columns, 1); p->columns=NULL; } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct tableparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct tableparams *p) { /* Free the allocated arrays: */ free(p->cp.hdu); free(p->cp.output); gal_list_data_free(p->table); } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/main.c�����������������������������������������������������������������������0000644�0001750�0001750�00000003142�13121462410�013062� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Table - View and manipulate a FITS table structures. Table is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" /* needs main.h. */ #include "table.h" /* needs main.h. */ /* Main function */ int main (int argc, char *argv[]) { struct tableparams p={{{0},0},0}; /* Set they starting time. */ time(&p.rawtime); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ table(&p); /* Free all non-freed allocations. */ ui_free_report(&p); /* Return successfully.*/ return EXIT_SUCCESS; } ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/Makefile.in������������������������������������������������������������������0000644�0001750�0001750�00000211251�13217217706�014055� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; \ elif test -n '$(MAKE_HOST)'; then \ true; \ elif test -n '$(MAKE_VERSION)' && test -n '$(CURDIR)'; then \ true; \ else \ false; \ fi; \ } am__make_running_with_option = \ case $${target_option-} in \ ?) ;; \ *) echo "am__make_running_with_option: internal error: invalid" \ "target option '$${target_option-}' specified" >&2; \ exit 1;; \ esac; \ has_opt=no; \ sane_makeflags=$$MAKEFLAGS; \ if $(am__is_gnu_make); 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@GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BIND = @GNULIB_BIND@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME 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uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/asttable.conf����������������������������������������������������������������0000644�0001750�0001750�00000001577�13121462410�014452� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Table. # Table is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ asttable --help # Full list of options, short doc. # $ asttable -P # Print all options and used values. # $ info asttable # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. ���������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/table/Makefile.am������������������������������������������������������������������0000644�0001750�0001750�00000002560�13121462410�014031� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2016, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = asttable asttable_LDADD = -lgnuastro asttable_SOURCES = main.c ui.c table.c EXTRA_DIST = main.h authors-cite.h args.h ui.h table.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = asttable.conf ������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220467�013167� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/statistics.h������������������������������������������������������������0000644�0001750�0001750�00000002104�13121462410�015435� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef STATISTICS_H #define STATISTICS_H void statistics(struct statisticsparams *p); #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/sky.h�������������������������������������������������������������������0000644�0001750�0001750�00000002057�13121462410�014060� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef SKY_H #define SKY_H void sky(struct statisticsparams *p); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/ui.h��������������������������������������������������������������������0000644�0001750�0001750�00000005262�13174462540�013704� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_SINGLE_VALUE = GAL_OPTIONS_GROUP_AFTER_COMMON, UI_GROUP_PARTICULAR_STAT, UI_GROUP_SKY, UI_GROUP_HIST_CFP, }; /* Available letters for short options: a b e f j p v w x z B G J L R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_COLUMN = 'c', UI_KEY_REFCOL = 'r', UI_KEY_GREATEREQUAL = 'g', UI_KEY_LESSTHAN = 'l', UI_KEY_QRANGE = 'Q', UI_KEY_MEAN = 'm', UI_KEY_STD = 'd', UI_KEY_MEDIAN = 'E', UI_KEY_MODE = 'O', UI_KEY_QUANTILE = 'u', UI_KEY_ASCIIHIST = 'A', UI_KEY_HISTOGRAM = 'H', UI_KEY_CUMULATIVE = 'C', UI_KEY_SIGMACLIP = 's', UI_KEY_NORMALIZE = 'n', UI_KEY_ONTILE = 't', UI_KEY_INTERPOLATE = 'i', UI_KEY_SKY = 'y', UI_KEY_KERNEL = 'k', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_NUMBER = 1000, UI_KEY_MINIMUM, UI_KEY_MAXIMUM, UI_KEY_SUM, UI_KEY_MODEQUANT, UI_KEY_MODESYM, UI_KEY_MODESYMVALUE, UI_KEY_QUANTFUNC, UI_KEY_ASCIICFP, UI_KEY_MIRROR, UI_KEY_NUMBINS, UI_KEY_NUMASCIIBINS, UI_KEY_ASCIIHEIGHT, UI_KEY_LOWERBIN, UI_KEY_ONEBINSTART, UI_KEY_MAXBINONE, UI_KEY_KHDU, UI_KEY_MIRRORDIST, UI_KEY_MODMEDQDIFF, UI_KEY_SMOOTHWIDTH, UI_KEY_CHECKSKY, UI_KEY_SCLIPPARAMS, }; /* Functions */ void ui_read_check_inputs_setup(int argc, char *argv[], struct statisticsparams *p); void ui_free_report(struct statisticsparams *p); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/args.h������������������������������������������������������������������0000644�0001750�0001750�00000033142�13174462540�014221� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { { "column", UI_KEY_COLUMN, "STR", 0, "Column name or number if input is a table.", GAL_OPTIONS_GROUP_INPUT, &p->column, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "refcol", UI_KEY_REFCOL, "STR", 0, "Reference column name or number.", GAL_OPTIONS_GROUP_INPUT, &p->refcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "greaterequal", UI_KEY_GREATEREQUAL, "FLT", 0, "Only use values greater-equal than this.", GAL_OPTIONS_GROUP_INPUT, &p->greaterequal, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "lessthan", UI_KEY_LESSTHAN, "FLT", 0, "Only use values less than this.", GAL_OPTIONS_GROUP_INPUT, &p->lessthan, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "qrange", UI_KEY_QRANGE, "FLT[,FLT]", 0, "Quantile range: one (from Q to 1-Q) or two.", GAL_OPTIONS_GROUP_INPUT, NULL, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_read_quantile_range }, /* Tessellation */ { "interpolate", UI_KEY_INTERPOLATE, 0, 0, "Interpolate over blank tiles to fill them.", GAL_OPTIONS_GROUP_TESSELLATION, &p->interpolate, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Single value measurements", UI_GROUP_SINGLE_VALUE }, { "number", UI_KEY_NUMBER, 0, 0, "Number (non-blank).", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "minimum", UI_KEY_MINIMUM, 0, 0, "Minimum.", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "maximum", UI_KEY_MAXIMUM, 0, 0, "Maximum.", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "sum", UI_KEY_SUM, 0, 0, "Sum.", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "mean", UI_KEY_MEAN, 0, 0, "Mean.", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "std", UI_KEY_STD, 0, 0, "Standad deviation.", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "median", UI_KEY_MEDIAN, 0, 0, "Median.", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "quantile", UI_KEY_QUANTILE, "FLT[,...]", 0, "Quantile (multiple values acceptable).", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "quantfunc", UI_KEY_QUANTFUNC, "FLT[,...]", 0, "Quantile function (multiple values acceptable).", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "mode", UI_KEY_MODE, 0, 0, "Mode (Appendix C of arXiv:1505.01664).", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "modequant", UI_KEY_MODEQUANT, 0, 0, "Mode quantile (see --mode)", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "modesym", UI_KEY_MODESYM, 0, 0, "Mode symmetricity (see --mode).", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { "modesymvalue", UI_KEY_MODESYMVALUE, 0, 0, "Value at mode symmetricity (see --mode).", UI_GROUP_SINGLE_VALUE, &p->singlevalue, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value }, { 0, 0, 0, 0, "Particular calculation", UI_GROUP_PARTICULAR_STAT }, { "asciihist", UI_KEY_ASCIIHIST, 0, 0, "Print an ASCII histogram.", UI_GROUP_PARTICULAR_STAT, &p->asciihist, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "asciicfp", UI_KEY_ASCIICFP, 0, 0, "Print an ASCII cumulative frequency plot.", UI_GROUP_PARTICULAR_STAT, &p->asciicfp, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "histogram", UI_KEY_HISTOGRAM, 0, 0, "Save the histogram in output.", UI_GROUP_PARTICULAR_STAT, &p->histogram, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "cumulative", UI_KEY_CUMULATIVE, 0, 0, "Save the cumulative frequency plot in output.", UI_GROUP_PARTICULAR_STAT, &p->cumulative, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "mirror", UI_KEY_MIRROR, "FLT", 0, "Save the histogram and CFP of the mirror dist.", UI_GROUP_PARTICULAR_STAT, &p->mirror, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "ontile", UI_KEY_ONTILE, 0, 0, "Single values on separate tiles, not full input.", UI_GROUP_PARTICULAR_STAT, &p->ontile, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "sky", UI_KEY_SKY, 0, 0, "Find the Sky and its STD over the tessellation.", UI_GROUP_PARTICULAR_STAT, &p->sky, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "sigmaclip", UI_KEY_SIGMACLIP, 0, 0, "Overall sigma-clipping (see `--sclipparams')", UI_GROUP_PARTICULAR_STAT, &p->sigmaclip, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Sky and Sky STD settings", UI_GROUP_SKY }, { "kernel", UI_KEY_KERNEL, "STR", 0, "File name of kernel to convolve input.", UI_GROUP_SKY, &p->kernelname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "khdu", UI_KEY_KHDU, "STR", 0, "HDU/extension name or number of kernel.", UI_GROUP_SKY, &p->khdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "mirrordist", UI_KEY_MIRRORDIST, "FLT", 0, "Max. distance (error multip.) to find mode.", UI_GROUP_SKY, &p->mirrordist, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "modmedqdiff", UI_KEY_MODMEDQDIFF, "FLT", 0, "Max. mode and median quantile diff. per tile.", UI_GROUP_SKY, &p->modmedqdiff, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "sclipparams", UI_KEY_SCLIPPARAMS, "FLT,FLT", 0, "Sigma clip: Multiple, and tolerance/number.", UI_GROUP_SKY, p->sclipparams, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_read_sigma_clip }, { "smoothwidth", UI_KEY_SMOOTHWIDTH, "INT", 0, "Sky: flat kernel width to smooth interpolated.", UI_GROUP_SKY, &p->smoothwidth, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_0_OR_ODD, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checksky", UI_KEY_CHECKSKY, 0, 0, "Store steps in `_sky_steps.fits' file.", UI_GROUP_SKY, &p->checksky, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Histogram and CFP settings", UI_GROUP_HIST_CFP }, { "numbins", UI_KEY_NUMBINS, "INT", 0, "No. of bins in histogram or CFP tables.", UI_GROUP_HIST_CFP, &p->numbins, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "numasciibins", UI_KEY_NUMASCIIBINS, "INT", 0, "No. of bins in ASCII histogram or CFP plots.", UI_GROUP_HIST_CFP, &p->numasciibins, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "asciiheight", UI_KEY_ASCIIHEIGHT, "INT", 0, "Height of ASCII histogram or CFP plots.", UI_GROUP_HIST_CFP, &p->asciiheight, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "normalize", UI_KEY_NORMALIZE, 0, 0, "Set sum of all bins to 1.", UI_GROUP_HIST_CFP, &p->normalize, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "maxbinone", UI_KEY_MAXBINONE, 0, 0, "Scale such that the maximum bin has value of one.", UI_GROUP_HIST_CFP, &p->maxbinone, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "onebinstart", UI_KEY_ONEBINSTART, "FLT", 0, "Shift bins so one bin starts on this value.", UI_GROUP_HIST_CFP, &p->onebinstart, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/authors-cite.h����������������������������������������������������������0000644�0001750�0001750�00000002773�13211076737�015703� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif �����gnuastro-0.5/bin/statistics/main.h������������������������������������������������������������������0000644�0001750�0001750�00000012010�13121462410�014164� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "Statistics" /* Program full name. */ #define PROGRAM_EXEC "aststatistics" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Input formats. */ enum statistics_input_format { INPUT_FORMAT_INVALID, INPUT_FORMAT_TABLE, INPUT_FORMAT_IMAGE, }; /* Main program parameters structure */ struct statisticsparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ gal_list_i32_t *singlevalue; /* Single value calculations. */ gal_list_f64_t *tp_args; /* Arguments for printing. */ char *inputname; /* Input filename. */ char *column; /* Column name or number if input is table. */ char *refcol; /* Reference column name or number. */ float greaterequal; /* Only use values >= this value. */ float lessthan; /* Only use values < this value. */ float quantmin; /* Quantile min or range: from Q to 1-Q. */ float quantmax; /* Quantile maximum. */ uint8_t ontile; /* Do single value calculations on tiles. */ uint8_t interpolate; /* Use interpolation to fill blank tiles. */ uint8_t asciihist; /* Print an ASCII histogram. */ uint8_t asciicfp; /* Print an ASCII cumulative frequency plot.*/ uint8_t histogram; /* Save histogram in output. */ uint8_t cumulative; /* Save cumulative distibution in output. */ double mirror; /* Mirror value for hist and CFP. */ uint8_t sky; /* Find the Sky value over the image. */ uint8_t sigmaclip; /* So sigma-clipping over all dataset. */ size_t numbins; /* Number of bins in histogram or CFP. */ size_t numasciibins; /* Number of bins in ASCII plots. */ size_t asciiheight; /* Height of ASCII histogram or CFP plots. */ uint8_t normalize; /* set the sum of all bins to 1. */ float onebinstart; /* Shift bins to start at this value. */ uint8_t maxbinone; /* Set the maximum bin to 1. */ float mirrordist; /* Maximum distance after mirror for mode. */ char *kernelname; /* File name of kernel to convolve input. */ char *khdu; /* Kernel HDU. */ float modmedqdiff; /* Mode and median quantile difference. */ size_t smoothwidth; /* Width of flat kernel to smooth interpd. */ uint8_t checksky; /* Save the steps for deriving the Sky. */ double sclipparams[2]; /* Muliple and parameter of sigma clipping. */ /* Internal */ uint8_t inputformat; /* Format of input dataset. */ int numoutfiles; /* Number of output files made in this run. */ uint8_t needssort; /* If sorting is needed. */ gal_data_t *input; /* Input data structure. */ gal_data_t *sorted; /* Sorted input data structure. */ gal_data_t *reference; /* Reference data structure. */ int isfits; /* Input is a FITS file. */ int hdu_type; /* Type of HDU (image or table). */ gal_data_t *kernel; /* Kernel for convolution of input for Sky. */ gal_data_t *convolved; /* Convolved input. */ gal_data_t *sky_t; /* Sky on each tile. */ gal_data_t *std_t; /* Sky standard deviation on each tile. */ char *checkskyname; /* Name of file for Sky calculation steps. */ time_t rawtime; /* Starting time of the program. */ }; #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/statistics.c������������������������������������������������������������0000644�0001750�0001750�00000066543�13175442274�015470� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <errno.h> #include <error.h> #include <float.h> #include <stdio.h> #include <string.h> #include <stdlib.h> #include <gnuastro/fits.h> #include <gnuastro/tile.h> #include <gnuastro/blank.h> #include <gnuastro/arithmetic.h> #include <gnuastro/statistics.h> #include <gnuastro/interpolate.h> #include <gnuastro/permutation.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "ui.h" #include "sky.h" #include "statistics.h" /*******************************************************************/ /************** Print in one row ***************/ /*******************************************************************/ static gal_data_t * statistics_pull_out_element(gal_data_t *input, size_t index) { size_t dsize=1; gal_data_t *out=gal_data_alloc(NULL, input->type, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); memcpy( out->array, gal_data_ptr_increment(input->array, index, input->type), gal_type_sizeof(input->type) ); return out; } static double statistics_read_check_args(struct statisticsparams *p) { double d; if(p->tp_args==NULL) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "address the problem. Not enough arguments for the requested " "single measurement options", __func__, PACKAGE_BUGREPORT); d=gal_list_f64_pop(&p->tp_args); return d; } static void statistics_print_one_row(struct statisticsparams *p) { int mustfree; char *toprint; size_t dsize=1; double arg, *d; gal_list_i32_t *tmp; gal_data_t *tmpv, *out=NULL, *num=NULL, *min=NULL, *max=NULL; gal_data_t *sum=NULL, *med=NULL, *meanstd=NULL, *modearr=NULL; /* The user can ask for any of the operators more than once, also some operators might return more than one usable value (like mode). So we will calculate the desired values once, and then print them. */ for(tmp=p->singlevalue; tmp!=NULL; tmp=tmp->next) switch(tmp->v) { /* Calculate respective values. Checking with `if(num==NULL)' gives compiler warnings of `this if clause does not guard ...'. So we are using this empty-if and else statement. */ case UI_KEY_NUMBER: num = num ? num : gal_statistics_number(p->input); break; case UI_KEY_MINIMUM: min = min ? min : gal_statistics_minimum(p->input); break; case UI_KEY_MAXIMUM: max = max ? max : gal_statistics_maximum(p->input); break; case UI_KEY_SUM: sum = sum ? sum : gal_statistics_sum(p->input); break; case UI_KEY_MEDIAN: med = med ? med : gal_statistics_median(p->sorted, 0); break; case UI_KEY_MEAN: case UI_KEY_STD: meanstd = meanstd ? meanstd : gal_statistics_mean_std(p->input); break; case UI_KEY_MODE: case UI_KEY_MODEQUANT: case UI_KEY_MODESYM: case UI_KEY_MODESYMVALUE: modearr = ( modearr ? modearr : gal_statistics_mode(p->sorted, p->mirrordist, 0) ); d=modearr->array; if(d[2]<GAL_STATISTICS_MODE_GOOD_SYM) d[0]=d[1]=NAN; break; /* Will be calculated as printed. */ case UI_KEY_QUANTILE: case UI_KEY_QUANTFUNC: break; /* The option isn't recognized. */ default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we " "can address the problem. Operation code %d not recognized", __func__, PACKAGE_BUGREPORT, tmp->v); } /* Print every requested number. */ for(tmp=p->singlevalue; tmp!=NULL; tmp=tmp->next) { /* By default don't free anything. */ mustfree=0; /* Get the output. */ switch(tmp->v) { /* Previously calculated values. */ case UI_KEY_NUMBER: out=num; break; case UI_KEY_MINIMUM: out=min; break; case UI_KEY_MAXIMUM: out=max; break; case UI_KEY_SUM: out=sum; break; case UI_KEY_MEDIAN: out=med; break; case UI_KEY_MEAN: out=statistics_pull_out_element(meanstd, 0); mustfree=1; break; case UI_KEY_STD: out=statistics_pull_out_element(meanstd, 1); mustfree=1; break; case UI_KEY_MODE: out=statistics_pull_out_element(modearr, 0); mustfree=1; break; case UI_KEY_MODEQUANT: out=statistics_pull_out_element(modearr, 1); mustfree=1; break; case UI_KEY_MODESYM: out=statistics_pull_out_element(modearr, 2); mustfree=1; break; case UI_KEY_MODESYMVALUE: out=statistics_pull_out_element(modearr, 3); mustfree=1; break; /* Not previously calculated. */ case UI_KEY_QUANTILE: arg = statistics_read_check_args(p); out = gal_statistics_quantile(p->sorted, arg, 0); break; case UI_KEY_QUANTFUNC: arg = statistics_read_check_args(p); tmpv = gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); *((double *)(tmpv->array)) = arg; tmpv = gal_data_copy_to_new_type_free(tmpv, p->input->type); out = gal_statistics_quantile_function(p->sorted, tmpv, 0); break; } /* Print the number. */ toprint=gal_type_to_string(out->array, out->type, 0); printf("%s ", toprint); free(toprint); /* Clean up (if necessary). */ if(mustfree) gal_data_free(out); } /* Print a new line. */ printf("\n"); /* Clean any of the allocated arrays. */ if(num) gal_data_free(num); if(min) gal_data_free(min); if(max) gal_data_free(max); if(sum) gal_data_free(sum); if(med) gal_data_free(med); if(meanstd) gal_data_free(meanstd); if(modearr) gal_data_free(modearr); } /*******************************************************************/ /************** Single value on tile ***************/ /*******************************************************************/ static void statistics_interpolate_and_write(struct statisticsparams *p, gal_data_t *values, char *output) { gal_data_t *interpd; struct gal_options_common_params *cp=&p->cp; /* Do the interpolation (if necessary). */ if( p->interpolate && !(p->cp.interponlyblank && gal_blank_present(values, 1)==0) ) { interpd=gal_interpolate_close_neighbors(values, &cp->tl, cp->interpnumngb, cp->numthreads, cp->interponlyblank, 0); gal_data_free(values); values=interpd; } /* Write the values. */ gal_tile_full_values_write(values, &cp->tl, 1, output, NULL, PROGRAM_NAME); } static void statistics_on_tile(struct statisticsparams *p) { double arg=0; gal_list_i32_t *operation; gal_data_t *tile, *values; size_t tind, dsize=1, mind=-1; uint8_t type=GAL_TYPE_INVALID; gal_data_t *tmp=NULL, *tmpv=NULL, *ttmp; struct gal_options_common_params *cp=&p->cp; struct gal_tile_two_layer_params *tl=&p->cp.tl; char *output=gal_checkset_automatic_output(cp, cp->output ? cp->output : p->inputname, "_ontile.fits"); /* Do the operation on each tile. */ for(operation=p->singlevalue; operation!=NULL; operation=operation->next) { /* Set the type of the output array. */ switch(operation->v) { case UI_KEY_NUMBER: type=GAL_TYPE_INT32; break; case UI_KEY_MINIMUM: case UI_KEY_MAXIMUM: case UI_KEY_MEDIAN: case UI_KEY_MODE: case UI_KEY_QUANTFUNC: type=p->input->type; break; case UI_KEY_SUM: case UI_KEY_MEAN: case UI_KEY_STD: case UI_KEY_QUANTILE: case UI_KEY_MODEQUANT: case UI_KEY_MODESYM: case UI_KEY_MODESYMVALUE: type=GAL_TYPE_FLOAT64; break; default: error(EXIT_FAILURE, 0, "%s: a bug! %d is not a recognized operation " "code", __func__, operation->v); } /* Allocate the space necessary to keep the value for each tile. */ values=gal_data_alloc(NULL, type, p->input->ndim, tl->numtiles, NULL, 0, p->input->minmapsize, NULL, NULL, NULL); /* Read the argument for those operations that need it. This is done here, because below, the functions are repeated on each tile. */ switch(operation->v) { case UI_KEY_QUANTILE: arg = statistics_read_check_args(p); break; case UI_KEY_QUANTFUNC: arg = statistics_read_check_args(p); tmpv = gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); *((double *)(tmpv->array)) = arg; tmpv = gal_data_copy_to_new_type_free(tmpv, p->input->type); } /* Do the operation on each tile. */ tind=0; for(tile=tl->tiles; tile!=NULL; tile=tile->next) { /* Do the proper operation. */ switch(operation->v) { case UI_KEY_NUMBER: tmp=gal_statistics_number(tile); break; case UI_KEY_MINIMUM: tmp=gal_statistics_minimum(tile); break; case UI_KEY_MAXIMUM: tmp=gal_statistics_maximum(tile); break; case UI_KEY_MEDIAN: tmp=gal_statistics_median(tile, 1); break; case UI_KEY_QUANTFUNC: tmp=gal_statistics_quantile_function(tile, tmpv, 1); break; case UI_KEY_SUM: tmp=gal_statistics_sum(tile); break; case UI_KEY_MEAN: tmp=gal_statistics_mean(tile); break; case UI_KEY_STD: tmp=gal_statistics_std(tile); break; case UI_KEY_QUANTILE: tmp=gal_statistics_quantile(tile, arg, 1); break; case UI_KEY_MODE: case UI_KEY_MODESYM: case UI_KEY_MODEQUANT: case UI_KEY_MODESYMVALUE: switch(operation->v) { case UI_KEY_MODE: mind=0; break; case UI_KEY_MODESYM: mind=2; break; case UI_KEY_MODEQUANT: mind=1; break; case UI_KEY_MODESYMVALUE: mind=3; break; } tmp=gal_statistics_mode(tile, p->mirrordist, 1); ttmp=statistics_pull_out_element(tmp, mind); gal_data_free(tmp); tmp=ttmp; break; default: error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to " "fix the problem. The operation code %d is not " "recognized", __func__, PACKAGE_BUGREPORT, operation->v); } /* Put the output value into the `values' array and clean up. */ tmp=gal_data_copy_to_new_type_free(tmp, type); memcpy(gal_data_ptr_increment(values->array, tind++, values->type), tmp->array, gal_type_sizeof(type)); gal_data_free(tmp); } /* Do the interpolation (if necessary) and write the array into the output. */ statistics_interpolate_and_write(p, values, output); /* Clean up. */ gal_data_free(values); if(operation->v==UI_KEY_QUANTFUNC) gal_data_free(tmpv); } /* Clean up. */ free(output); } /*******************************************************************/ /************** ASCII plots ***************/ /*******************************************************************/ static void print_ascii_plot(struct statisticsparams *p, gal_data_t *plot, gal_data_t *bins, int h1_c0, int printinfo) { int i, j; size_t *s, *sf, max=0; double *b, v, halfbinwidth, correction; /* Find the maximum of the plot. */ sf=(s=plot->array)+plot->size; do max = *s>max ? *s : max; while(++s<sf); /* Print the range so the user knows. */ if(printinfo) { b=bins->array; halfbinwidth = (b[1]-b[0])/2; printf("\nASCII %s:\n", ( h1_c0 ? "Histogram" : "Cumulative frequency plot") ); if(h1_c0) printf("Number: %zu\n", p->input->size); printf("Y: (linear: 0 to %zu)\n", max); printf("X: (linear: %g -- %g, in %zu bins)\n", b[0]-halfbinwidth, b[ bins->size - 1 ] + halfbinwidth, bins->size); } /* Print the ASCII plot: */ s=plot->array; correction = (double)(p->asciiheight) / (double)max; for(i=p->asciiheight;i>=0;--i) { printf(" |"); for(j=0;j<plot->size;++j) { v = (double)s[j] * correction; if( v >= ((double)i-0.5f) && v > 0.0f ) printf("*"); else printf(" "); } printf("\n"); } printf(" |"); for(j=0;j<plot->size;++j) printf("-"); printf("\n\n"); } static void ascii_plots(struct statisticsparams *p) { gal_data_t *bins, *hist, *cfp=NULL; /* Make the bins and the respective plot. */ bins=gal_statistics_regular_bins(p->input, NULL, p->numasciibins, NAN); hist=gal_statistics_histogram(p->input, bins, 0, 0); if(p->asciicfp) { bins->next=hist; cfp=gal_statistics_cfp(p->input, bins, 0); } /* Print the plots. */ if(p->asciihist) print_ascii_plot(p, hist, bins, 1, 1); if(p->asciicfp) print_ascii_plot(p, cfp, bins, 0, 1); /* Clean up.*/ gal_data_free(bins); gal_data_free(hist); if(p->asciicfp) gal_data_free(cfp); } /*******************************************************************/ /******* Histogram and cumulative frequency tables ***********/ /*******************************************************************/ void write_output_table(struct statisticsparams *p, gal_data_t *table, char *suf, char *contents) { char *output; int use_auto_output=0; char *fix, *suffix=NULL, *tmp; gal_list_str_t *comments=NULL; /* Automatic output should be used when no output name was specified or we have more than one output file. */ use_auto_output = p->cp.output ? (p->numoutfiles>1 ? 1 : 0) : 1; /* Set the `fix' and `suffix' strings. Note that `fix' is necessary in every case, even when no automatic output is to be used. Since it is used to determine the format of the output. */ fix = ( p->cp.output ? gal_fits_name_is_fits(p->cp.output) ? "fits" : "txt" : "txt" ); if(use_auto_output) asprintf(&suffix, "%s.%s", suf, fix); /* Make the output name. */ output = ( use_auto_output ? gal_checkset_automatic_output(&p->cp, p->inputname, suffix) : p->cp.output ); /* Write the comments, NOTE: we are writing the first two in reverse of the order we want them. They will later be freed as part of the list's freeing.*/ tmp=gal_fits_name_save_as_string(p->inputname, p->cp.hdu); gal_list_str_add(&comments, tmp, 0); asprintf(&tmp, "%s created from:", contents); gal_list_str_add(&comments, tmp, 0); if(strcmp(fix, "fits")) /* The intro info will be in FITS files anyway.*/ gal_table_comments_add_intro(&comments, PROGRAM_NAME, &p->rawtime); /* Write the table. */ gal_checkset_writable_remove(output, 0, p->cp.dontdelete); gal_table_write(table, comments, p->cp.tableformat, output, "TABLE"); /* Let the user know, if we aren't in quiet mode. */ if(!p->cp.quiet) printf("%s created.\n", output); /* Clean up. */ if(suffix) free(suffix); gal_list_str_free(comments, 1); if(output!=p->cp.output) free(output); } static void save_hist_and_or_cfp(struct statisticsparams *p) { char *suf, *contents; gal_data_t *bins, *hist, *cfp=NULL; /* Set the bins and make the histogram, this is necessary for both the histogram and CFP (recall that the CFP is built from the histogram). */ bins=gal_statistics_regular_bins(p->input, NULL, p->numbins, p->onebinstart); hist=gal_statistics_histogram(p->input, bins, p->normalize, p->maxbinone); /* Set the histogram as the next pointer of bins. This is again necessary in both cases: when only a histogram is requested, it is used for the plotting. When only a CFP is desired, it is used as input into `gal_statistics_cfp'. */ bins->next=hist; /* Make the cumulative frequency plot if the user wanted it. Make the CFP, note that for the CFP, `maxbinone' and `normalize' are the same: the last bin (largest value) must be one. So if any of them are given, then set the last argument to 1.*/ if(p->cumulative) cfp=gal_statistics_cfp(p->input, bins, p->normalize || p->maxbinone); /* FITS tables don't accept `uint64_t', so to be consistent, we'll conver the histogram and CFP to `uint32_t'.*/ if(hist->type==GAL_TYPE_UINT64) hist=gal_data_copy_to_new_type_free(hist, GAL_TYPE_UINT32); if(cfp && cfp->type==GAL_TYPE_UINT64) cfp=gal_data_copy_to_new_type_free(cfp, GAL_TYPE_UINT32); /* Finalize the next pointers. */ bins->next=hist; hist->next=cfp; /* Prepare the contents. */ if(p->histogram && p->cumulative) { suf="_hist_cfp"; contents="Histogram and cumulative frequency plot"; } else if(p->histogram) { suf="_hist"; contents="Histogram"; } else { suf="_cfp"; contents="Cumulative frequency plot"; } /* Set the output file name. */ write_output_table(p, bins, suf, contents); } void print_mirror_hist_cfp(struct statisticsparams *p) { size_t dsize=1; gal_data_t *table; double mirror_val; gal_data_t *mirror=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 1, -1, NULL, NULL, NULL); /* Convert the given mirror value into the type of the input dataset. */ *((double *)(mirror->array)) = p->mirror; mirror=gal_data_copy_to_new_type_free(mirror, p->input->type); /* Make the table columns. */ table=gal_statistics_mode_mirror_plots(p->sorted, mirror, p->numbins, 0, &mirror_val); if(p->mirror!=mirror_val) { fprintf(stderr, "Warning: Mirror value is %f.\n", mirror_val); if(!p->cp.quiet) fprintf(stderr, "\nNote that the mirror distribution is discrete " "and depends on the input data. So the closest point in " "the data to your desired mirror at %f was %f.\n\n", p->mirror, mirror_val); } /* If the mirror value was out-of-range, then no table will be made. */ if(table) write_output_table(p, table, "_mirror_hist_cfp", "Histogram and CFP of mirror distribution"); else error(EXIT_FAILURE, 0, "%s: mirror value %g is out of range", __func__, p->mirror); } /*******************************************************************/ /************** Basic information ***************/ /*******************************************************************/ /* To keep things in `print_basics' clean, we'll define the input data here, then only print the values there. */ void print_input_info(struct statisticsparams *p) { char *str, *name, *col=NULL; /* Print the program name and version. */ printf("%s\n", PROGRAM_NAME); /* Print the input information, if the input was a table, we also need to give the column information. When the column has a name, it will be printed, when it doesn't, we'll use the same string the user gave. */ printf("-------\n"); name=gal_fits_name_save_as_string(p->inputname, p->cp.hdu); printf("Input: %s\n", name); /* If a table was given, print the column. */ if(p->column) printf("Column: %s\n", p->input->name ? p->input->name : p->column); /* Range. */ str=NULL; if( !isnan(p->greaterequal) && !isnan(p->lessthan) ) asprintf(&str, "from (inclusive) %g, up to (exclusive) %g", p->greaterequal, p->lessthan); else if( !isnan(p->greaterequal) ) asprintf(&str, "from (inclusive) %g", p->greaterequal); else if( !isnan(p->lessthan) ) asprintf(&str, "up to (exclusive) %g", p->lessthan); if(str) { printf("Range: "); if(p->refcol) printf("[on column %s] ", p->reference->name ? p->reference->name : p->refcol); printf("%s.\n", str); free(str); } /* Units. */ if(p->input->unit) printf("Unit: %s\n", p->input->unit); /* Clean up. */ if(col) free(col); free(name); printf("-------\n"); } /* This function will report the simple immediate statistics of the data. For the average and standard deviation, the unsorted data is used so we don't suddenly encounter rounding errors. */ void print_basics(struct statisticsparams *p) { char *str; int namewidth=40; float mirrdist=1.5; double mean, std, *d; gal_data_t *tmp, *bins, *hist; /* Define the input dataset. */ print_input_info(p); /* Print the number: */ printf(" %-*s %zu\n", namewidth, "Number of elements:", p->input->size); /* Minimum: */ tmp=gal_statistics_minimum(p->input); str=gal_type_to_string(tmp->array, tmp->type, 0); printf(" %-*s %s\n", namewidth, "Minimum:", str); gal_data_free(tmp); free(str); /* Maximum: */ tmp=gal_statistics_maximum(p->input); str=gal_type_to_string(tmp->array, tmp->type, 0); printf(" %-*s %s\n", namewidth, "Maximum:", str); gal_data_free(tmp); free(str); /* Find the mean and standard deviation, but don't print them, see explanations under median. */ tmp=gal_statistics_mean_std(p->input); mean = ((double *)(tmp->array))[0]; std = ((double *)(tmp->array))[1]; gal_data_free(tmp); /* Mode of the distribution (if it is valid). we want the mode and median to be found in place to save time/memory. But having a sorted array can decrease the floating point accuracy of the standard deviation. So we'll do the median calculation in the end.*/ tmp=gal_statistics_mode(p->input, mirrdist, 1); d=tmp->array; if(d[2]>GAL_STATISTICS_MODE_GOOD_SYM) { /* Same format as `gal_data_write_to_string' */ printf(" %-*s %.10g\n", namewidth, "Mode:", d[0]); printf(" %-*s %.10g\n", namewidth, "Mode quantile:", d[1]); } gal_data_free(tmp); /* Find and print the median: */ tmp=gal_statistics_median(p->input, 0); str=gal_type_to_string(tmp->array, tmp->type, 0); printf(" %-*s %s\n", namewidth, "Median:", str); gal_data_free(tmp); free(str); /* Print the mean and standard deviation. Same format as `gal_data_write_to_string' */ printf(" %-*s %.10g\n", namewidth, "Mean:", mean); printf(" %-*s %.10g\n", namewidth, "Standard deviation:", std); /* Ascii histogram. Note that we don't want to force the user to have the plotting parameters. Also, when a reference column is defined, the range shown in the basic information section applies to that, not the range of the histogram. In that case, we want to print the histogram information. */ printf("-------"); p->asciiheight = p->asciiheight ? p->asciiheight : 10; p->numasciibins = p->numasciibins ? p->numasciibins : 70; bins=gal_statistics_regular_bins(p->input, NULL, p->numasciibins, NAN); hist=gal_statistics_histogram(p->input, bins, 0, 0); if(p->refcol==NULL) printf("\nHistogram:\n"); print_ascii_plot(p, hist, bins, 1, p->refcol ? 1 : 0); gal_data_free(bins); gal_data_free(hist); } /*******************************************************************/ /************** Sigma clipping ***************/ /*******************************************************************/ void print_sigma_clip(struct statisticsparams *p) { float *a; char *mode; int namewidth=40; gal_data_t *sigclip; /* Set the mode for printing: */ if( p->sclipparams[1]>=1.0f ) asprintf(&mode, "for %g clips", p->sclipparams[1]); else asprintf(&mode, "until relative change in STD is less than %g", p->sclipparams[1]); /* Report the status */ if(!p->cp.quiet) { print_input_info(p); printf("%g-sigma clipping steps %s:\n\n", p->sclipparams[0], mode); } /* Do the Sigma clipping: */ sigclip=gal_statistics_sigma_clip(p->sorted, p->sclipparams[0], p->sclipparams[1], 0, p->cp.quiet); a=sigclip->array; /* Finish the introduction. */ if(!p->cp.quiet) printf("-------\nSummary:\n"); else printf("%g-sigma clipped %s:\n", p->sclipparams[0], mode); /* Print the final results: */ printf(" %-*s %zu\n", namewidth, "Number of input elements:", p->input->size); if( p->sclipparams[1] < 1.0f ) printf(" %-*s %d\n", namewidth, "Number of clips:", sigclip->status); printf(" %-*s %.0f\n", namewidth, "Final number of elements:", a[0]); printf(" %-*s %g\n", namewidth, "Median:", a[1]); printf(" %-*s %g\n", namewidth, "Mean:", a[2]); printf(" %-*s %g\n", namewidth, "Standard deviation:", a[3]); /* Clean up. */ free(mode); } /*******************************************************************/ /************** Main function ***************/ /*******************************************************************/ void statistics(struct statisticsparams *p) { int print_basic_info=1; /* Print the one-row numbers if the user asked for them. */ if(p->singlevalue) { print_basic_info=0; if(p->ontile) statistics_on_tile(p); else statistics_print_one_row(p); } /* Find the Sky value if called. */ if(p->sky) { sky(p); print_basic_info=0; } /* Print the ASCII plots if requested. */ if(p->asciihist || p->asciicfp) { ascii_plots(p); print_basic_info=0; } /* Save the histogram and CFP as tables if requested. */ if(p->histogram || p->cumulative) { print_basic_info=0; save_hist_and_or_cfp(p); } /* Print the sigma-clipped results. */ if( p->sigmaclip ) { print_basic_info=0; print_sigma_clip(p); } /* Make the mirror table. */ if( !isnan(p->mirror) ) { print_basic_info=0; print_mirror_hist_cfp(p); } /* If nothing was requested print the simple statistics. */ if(print_basic_info) print_basics(p); } �������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/sky.c�������������������������������������������������������������������0000644�0001750�0001750�00000021751�13156610402�014061� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <gnuastro/fits.h> #include <gnuastro/qsort.h> #include <gnuastro/blank.h> #include <gnuastro/threads.h> #include <gnuastro/convolve.h> #include <gnuastro/statistics.h> #include <gnuastro/interpolate.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" static void * sky_on_thread(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct statisticsparams *p=(struct statisticsparams *)tprm->params; double *darr; int stype=p->sky_t->type; void *tblock=NULL, *tarray=NULL; gal_data_t *tile, *mode, *sigmaclip; size_t i, tind, twidth=gal_type_sizeof(stype); /* Find the Sky and its standard deviation on the tiles given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* Set the tile and copy its values into the array we'll be using. */ tind = tprm->indexs[i]; tile = &p->cp.tl.tiles[tind]; /* If we have a convolved image, temporarily (only for finding the mode) change the tile's pointers so we can work on the convolved image for the mode. */ if(p->kernel) { tarray=tile->array; tblock=tile->block; tile->array=gal_tile_block_relative_to_other(tile, p->convolved); tile->block=p->convolved; } mode=gal_statistics_mode(tile, p->mirrordist, 1); if(p->kernel) { tile->array=tarray; tile->block=tblock; } /* Check the mode value. Note that if the mode is in-accurate, then the values will be NaN and all conditionals will fail. So, we'll go onto finding values for this tile */ darr=mode->array; if( fabs(darr[1]-0.5f) < p->modmedqdiff ) { /* Get the sigma-clipped mean and standard deviation. `inplace' is irrelevant here because this is a tile and it will be copied anyway. */ sigmaclip=gal_statistics_sigma_clip(tile, p->sclipparams[0], p->sclipparams[1], 1, 1); /* Put the mean and its standard deviation into the respective place for this tile. */ sigmaclip=gal_data_copy_to_new_type_free(sigmaclip, stype); memcpy(gal_data_ptr_increment(p->sky_t->array, tind, stype), gal_data_ptr_increment(sigmaclip->array, 2, stype), twidth); memcpy(gal_data_ptr_increment(p->std_t->array, tind, stype), gal_data_ptr_increment(sigmaclip->array, 3, stype), twidth); /* Clean up. */ gal_data_free(sigmaclip); } else { gal_blank_write(gal_data_ptr_increment(p->sky_t->array, tind, stype), stype); gal_blank_write(gal_data_ptr_increment(p->std_t->array, tind, stype), stype); } /* Clean up. */ gal_data_free(mode); } /* Wait for all threads to finish and return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } void sky(struct statisticsparams *p) { char *msg, *outname; struct timeval t0, t1; gal_data_t *num, *tmp; struct gal_options_common_params *cp=&p->cp; struct gal_tile_two_layer_params *tl=&cp->tl; /* Print basic information */ if(!cp->quiet) { gettimeofday(&t0, NULL); printf("%s\n", PROGRAM_STRING); printf("Estimating Sky (reference value) and its STD.\n"); printf("-----------\n"); printf(" - Using %zu CPU thread%s.\n", cp->numthreads, cp->numthreads==1 ? "" : "s"); printf(" - Input: %s (hdu: %s)\n", p->inputname, cp->hdu); if(p->kernelname) printf(" - Kernel: %s (hdu: %s)\n", p->kernelname, p->khdu); } /* When checking steps, the input image is the first extension. */ if(p->checksky) gal_fits_img_write(p->input, p->checkskyname, NULL, PROGRAM_NAME); /* Convolve the image (if desired). */ if(p->kernel) { if(!cp->quiet) gettimeofday(&t1, NULL); p->convolved=gal_convolve_spatial(tl->tiles, p->kernel, cp->numthreads, 1, tl->workoverch); if(p->checksky) gal_fits_img_write(p->convolved, p->checkskyname, NULL, PROGRAM_NAME); if(!cp->quiet) gal_timing_report(&t1, "Input convolved with kernel.", 1); } /* Make the arrays keeping the Sky and Sky standard deviation values. */ p->sky_t=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, p->input->ndim, tl->numtiles, NULL, 0, p->input->minmapsize, "SKY", p->input->unit, NULL); p->std_t=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, p->input->ndim, tl->numtiles, NULL, 0, p->input->minmapsize, "SKY STD", p->input->unit, NULL); /* Find the Sky and Sky standard deviation on the tiles. */ if(!cp->quiet) gettimeofday(&t1, NULL); gal_threads_spin_off(sky_on_thread, p, tl->tottiles, cp->numthreads); if(!cp->quiet) { num=gal_statistics_number(p->sky_t); asprintf(&msg, "Sky and its STD found on %zu/%zu tiles.", (size_t)(*((uint64_t *)(num->array))), tl->tottiles ); gal_timing_report(&t1, msg, 1); gal_data_free(num); free(msg); } if(p->checksky) { gal_tile_full_values_write(p->sky_t, tl, 1, p->checkskyname, NULL, PROGRAM_NAME); gal_tile_full_values_write(p->std_t, tl, 1, p->checkskyname, NULL, PROGRAM_NAME); } /* Interpolate the Sky and its standard deviation. */ if(!cp->quiet) gettimeofday(&t1, NULL); p->sky_t->next=p->std_t; tmp=gal_interpolate_close_neighbors(p->sky_t, tl, cp->interpnumngb, cp->numthreads, cp->interponlyblank, 1); gal_data_free(p->sky_t); gal_data_free(p->std_t); p->sky_t=tmp; p->std_t=tmp->next; p->sky_t->next=p->std_t->next=NULL; if(!cp->quiet) gal_timing_report(&t1, "All blank tiles filled (interplated).", 1); if(p->checksky) { gal_tile_full_values_write(p->sky_t, tl, 1, p->checkskyname, NULL, PROGRAM_NAME); gal_tile_full_values_write(p->std_t, tl, 1, p->checkskyname, NULL, PROGRAM_NAME); } /* Smooth the Sky and Sky STD arrays. */ if(p->smoothwidth>1) { if(!cp->quiet) gettimeofday(&t1, NULL); tmp=gal_tile_full_values_smooth(p->sky_t, tl, p->smoothwidth, p->cp.numthreads); gal_data_free(p->sky_t); p->sky_t=tmp; tmp=gal_tile_full_values_smooth(p->std_t, tl, p->smoothwidth, p->cp.numthreads); gal_data_free(p->std_t); p->std_t=tmp; if(!cp->quiet) gal_timing_report(&t1, "Smoothed Sky and Sky STD values on tiles.", 1); if(p->checksky) { gal_tile_full_values_write(p->sky_t, tl, 1, p->checkskyname, NULL, PROGRAM_NAME); gal_tile_full_values_write(p->std_t, tl, 1, p->checkskyname, NULL, PROGRAM_NAME); } } /* Save the Sky and its standard deviation */ outname=gal_checkset_automatic_output(&p->cp, ( p->cp.output ? p->cp.output : p->inputname ), "_sky.fits"); gal_tile_full_values_write(p->sky_t, tl, 1, outname, NULL, PROGRAM_NAME); gal_tile_full_values_write(p->std_t, tl, 1, outname, NULL, PROGRAM_NAME); if(!cp->quiet) printf(" - Written to `%s'.\n", outname); /* Clean up and return. */ free(outname); gal_data_free(p->sky_t); gal_data_free(p->std_t); gal_data_free(p->convolved); if(!cp->quiet) { printf("-----------\n"); gal_timing_report(&t0, "Completed in:", 0); printf("-----------\n"); } } �����������������������gnuastro-0.5/bin/statistics/ui.c��������������������������������������������������������������������0000644�0001750�0001750�00000074346�13211616535�013705� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/tile.h> #include <gnuastro/qsort.h> #include <gnuastro/blank.h> #include <gnuastro/table.h> #include <gnuastro/threads.h> #include <gnuastro/arithmetic.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/tableintern.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will do statistical " "analysis on the input dataset (table column or image). All blank " "pixels or pixels outside of the given range are ignored. You can " "either directly ask for certain statistics in one line/row as shown " "below with the same order as requested, or get tables of different " "statistical measures like the histogram, cumulative frequency style " "and etc. If no particular statistic is requested, some basic " "information about the dataset is printed on the command-line.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct statisticsparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_struct = p; cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; cp->numthreads = gal_threads_number(); cp->tl.remainderfrac = NAN; /* Program-specific initializers */ p->lessthan = NAN; p->onebinstart = NAN; p->greaterequal = NAN; p->quantmin = NAN; p->quantmax = NAN; p->mirror = NAN; p->mirrordist = NAN; p->modmedqdiff = NAN; p->sclipparams[0] = NAN; p->sclipparams[1] = NAN; /* Set the mandatory common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_TYPE: cp->coptions[i].flags=OPTION_HIDDEN; break; case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_MINMAPSIZE: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct statisticsparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->inputname) argp_error(state, "only one argument (input file) should be given"); else p->inputname=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } static void * ui_add_to_single_value(struct argp_option *option, char *arg, char *filename, size_t lineno, void *params) { size_t i; double *d; gal_data_t *inputs=NULL; struct statisticsparams *p=(struct statisticsparams *)params; /* In case of printing the option values. */ if(lineno==-1) error(EXIT_FAILURE, 0, "currently the options to be printed in one row " "(like `--number', `--mean', and etc) do not support printing " "with the `--printparams' (`-P'), or writing into configuration " "files due to lack of time when implementing these features. " "You can put them into configuration files manually. Please get " "in touch with us at `%s', so we can implement it", PACKAGE_BUGREPORT); /* Some of these options take values and some don't. */ if(option->type==GAL_OPTIONS_NO_ARG_TYPE) { /* If this option is given in a configuration file, then `arg' will not be NULL and we don't want to do anything if it is `0'. */ if(arg) { /* Make sure the value is only `0' or `1'. */ if( arg[1]!='\0' && *arg!='0' && *arg!='1' ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the `--%s' " "option takes no arguments. In a configuration " "file it can only have the values `1' or `0', " "indicating if it should be used or not", option->name); /* Only proceed if the (possibly given) argument is 1. */ if(arg[0]=='0' && arg[1]=='\0') return NULL; } /* Add this option to the print list. */ gal_list_i32_add(&p->singlevalue, option->key); } else { /* Read the string of numbers. */ inputs=gal_options_parse_list_of_numbers(arg, filename, lineno); d=inputs->array; /* Do the appropriate operations with the */ switch(option->key) { case UI_KEY_QUANTILE: case UI_KEY_QUANTFUNC: /* For the quantile and the quantile function, its possible to give any number of arguments, so add the operation index and the argument once for each given number. */ for(i=0;i<inputs->size;++i) { if(option->key==UI_KEY_QUANTILE && (d[i]<0 || d[i]>1) ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "values " "to `--quantile' (`-u') must be between 0 " "and 1, you had asked for %g (read from `%s')", d[i], arg); gal_list_f64_add(&p->tp_args, d[i]); gal_list_i32_add(&p->singlevalue, option->key); } break; default: error_at_line(EXIT_FAILURE, 0, filename, lineno, "a bug! please " "contact us at %s so we can address the problem. " "the option given to `ui_add_to_print_in_row' is " "marked as requiring a value, but is not recognized", PACKAGE_BUGREPORT); } } return NULL; } static void * ui_read_quantile_range(struct argp_option *option, char *arg, char *filename, size_t lineno, void *params) { char *str; gal_data_t *in; struct statisticsparams *p=(struct statisticsparams *)params; /* For the `--printparams' (`-P') option:*/ if(lineno==-1) { if( isnan(p->quantmax) ) asprintf(&str, "%g", p->quantmin); else asprintf(&str, "%g,%g", p->quantmin, p->quantmax); return str; } /* Parse the inputs. */ in=gal_options_parse_list_of_numbers(arg, filename, lineno); /* Check if there was only two numbers. */ if(in->size!=1 && in->size!=2) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the `--%s' " "option takes one or two values values (separated by " "a comma) to define the range of used values with " "quantiles. However, %zu numbers were read in the " "string `%s' (value to this option).\n\n" "If there is only one number as input, it will be " "interpretted as the lower quantile (Q) range. The " "higher range will be set to the quantile (1-Q). " "When two numbers are given, they will be used as the " "lower and higher quantile range respectively", option->name, in->size, arg); /* Read the values in. */ p->quantmin = ((double *)(in->array))[0]; if(in->size==2) p->quantmax = ((double *)(in->array))[1]; /* Make sure the values are between 0 and 1. */ if( (p->quantmin<0 || p->quantmin>1) || ( !isnan(p->quantmax) && (p->quantmax<0 || p->quantmax>1) ) ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "values to the " "`--quantrange' option must be between 0 and 1 " "(inclusive). Your input was: `%s'", arg); /* When only one value is given, make sure it is less than 0.5. */ if( !isnan(p->quantmax) && p->quantmin>0.5 ) error(EXIT_FAILURE, 0, "%g>=0.5! When only one value is given to the " "`--%s' option, the range is defined as Q and 1-Q. Thus, the " "value must be less than 0.5", p->quantmin, option->name); /* Clean up and return. */ gal_data_free(in); return NULL; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct statisticsparams *p) { gal_list_i32_t *tmp; struct gal_tile_two_layer_params *tl=&p->cp.tl; /* Check if the format of the output table is valid, given the type of the output. */ gal_tableintern_check_fits_format(p->cp.output, p->cp.tableformat); /* If in tile-mode, we must have at least one single valued option. */ if(p->ontile && p->singlevalue==NULL) error(EXIT_FAILURE, 0, "at least one of the single-value measurements " "(for example `--median') must be requested with the `--ontile' " "option: there is no value to put in each tile"); /* Tessellation related options. */ if( p->ontile || p->sky ) { /* The tile or sky mode cannot be called with any other modes. */ if(p->asciihist || p->asciicfp || p->histogram || p->cumulative || p->sigmaclip || !isnan(p->mirror) ) error(EXIT_FAILURE, 0, "`--ontile' or `--sky' cannot be called with " "any of the `particular' calculation options, for example " "`--histogram'. This is because the latter work over the whole " "dataset and element positions are changed, but in the former " "positions are significant"); /* Make sure the tessellation defining options are given. */ if( tl->tilesize==NULL || tl->numchannels==NULL || isnan(tl->remainderfrac) ) error(EXIT_FAILURE, 0, "`--tilesize', `--numchannels', and " "`--remainderfrac' are mandatory options when dealing with " "a tessellation (in `--ontile' or `--sky' mode). Atleast " "one of these options wasn't given a value."); } /* In Sky mode, several options are mandatory. */ if( p->sky ) { /* Mandatory options. */ if ( isnan(p->modmedqdiff) || isnan(p->sclipparams[0]) || p->cp.interpnumngb==0 || isnan(p->mirrordist) ) error(EXIT_FAILURE, 0, "`--modmedqdiff', `--sclipparams', " "`--mirrordist', and `--interpnumngb' are mandatory with " "`--sky'"); /* If mode and median distance is a reasonable value. */ if(p->modmedqdiff>0.5) error(EXIT_FAILURE, 0, "%f not acceptable for `--modmedqdiff'. It " "cannot take values larger than 0.5 (quantile of median)", p->modmedqdiff); /* If a kernel name has been given, we need the HDU. */ if(p->kernelname && gal_fits_name_is_fits(p->kernelname) && p->khdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified for the kernel image. When " "A HDU is necessary for FITS files. You can use the `--khdu' " "(`-u') option and give it the HDU number (starting from " "zero), extension name, or anything acceptable by CFITSIO"); } /* Sigma-clipping needs `sclipparams'. */ if(p->sigmaclip && isnan(p->sclipparams[0])) error(EXIT_FAILURE, 0, "`--sclipparams' is necessary with `--sigmaclip'. " "`--sclipparams' takes two values (separated by a comma) for " "defining the sigma-clip: the multiple of sigma, and tolerance " "(<1) or number of clips (>1)."); /* If any of the mode measurements are requested, then `mirrordist' is mandatory. */ for(tmp=p->singlevalue; tmp!=NULL; tmp=tmp->next) switch(tmp->v) { case UI_KEY_MODE: case UI_KEY_MODESYM: case UI_KEY_MODEQUANT: case UI_KEY_MODESYMVALUE: if( isnan(p->mirrordist) ) error(EXIT_FAILURE, 0, "`--mirrordist' is required for the " "mode-related single measurements (`--mode', `--modequant', " "`--modesym', and `--modesymvalue')"); } /* If less than and greater than are both given, make sure that the value to greater than is smaller than the value to less-than. */ if( !isnan(p->lessthan) && !isnan(p->greaterequal) && p->lessthan < p->greaterequal ) error(EXIT_FAILURE, 0, "the value to `--lessthan' (%g) must be larger " "than the value to `--greaterequal' (%g)", p->lessthan, p->greaterequal); /* Less-than and greater-equal cannot be called together with quantrange. */ if( ( !isnan(p->lessthan) || !isnan(p->greaterequal) ) && !isnan(p->quantmin) ) error(EXIT_FAILURE, 0, "`--lessthan' and/or `--greaterequal' cannot " "be called together with `--quantrange'"); /* When binned outputs are requested, make sure that `numbins' is set. */ if( (p->histogram || p->cumulative || !isnan(p->mirror)) && p->numbins==0) error(EXIT_FAILURE, 0, "`--numbins' isn't set. When the histogram or " "cumulative frequency plots are requested, the number of bins " "(`--numbins') is necessary"); /* If an ascii plot is requested, check if the ascii number of bins and height are given. */ if( (p->asciihist || p->asciicfp) && (p->numasciibins==0 || p->asciiheight==0) ) error(EXIT_FAILURE, 0, "when an ascii plot is requested, " "`--numasciibins' and `--asciiheight' are mandatory, but atleast " "one of these has not been given"); /* Reverse the list of statistics to print in one row and also the arguments, so it has the same order the user wanted. */ gal_list_f64_reverse(&p->tp_args); gal_list_i32_reverse(&p->singlevalue); } static void ui_check_options_and_arguments(struct statisticsparams *p) { char *name=NULL; if(p->inputname) { /* If input is FITS. */ if( (p->isfits=gal_fits_name_is_fits(p->inputname)) ) { /* Check if a HDU is given. */ if( p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified. When the input is a " "FITS file, a HDU must also be specified, you can use " "the `--hdu' (`-h') option and give it the HDU number " "(starting from zero), extension name, or anything " "acceptable by CFITSIO"); /* If its a table, make sure a column is also specified. */ p->hdu_type=gal_fits_hdu_format(p->inputname, p->cp.hdu); if(p->hdu_type==IMAGE_HDU) { if(p->column) error(EXIT_FAILURE, 0, "%s (hdu: %s): is a FITS image " "extension. The `--column' option is only applicable " "to tables.", p->inputname, p->cp.hdu); } else if(p->column==NULL) asprintf(&name, "%s (hdu: %s)", p->inputname, p->cp.hdu); } /* If its not FITS, it must be a table. */ else { if(p->column==NULL) name=p->inputname; } /* If a column was necessary, but not given, print an error. */ if(name) error(EXIT_FAILURE, 0, "%s is a table but no column is " "specified. Please use the `--column' (`-c') option to " "specify a column.\n\nYou can either give it the column number " "(couting from 1), or a match/search in its meta-data (e.g., " "column names). For more information, please run the " "following command (press the `SPACE' key to go down and " "`q' to return to the command-line):\n\n" " $ info gnuastro \"Selecting table columns\"\n", name); } else error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ static void ui_out_of_range_to_blank(struct statisticsparams *p) { size_t one=1; unsigned char flags=GAL_ARITHMETIC_NUMOK; unsigned char flagsor = ( GAL_ARITHMETIC_FREE | GAL_ARITHMETIC_INPLACE | GAL_ARITHMETIC_NUMOK ); gal_data_t *tmp, *cond_g=NULL, *cond_l=NULL, *cond, *blank, *ref; /* Set the dataset that should be used for the condition. */ ref = p->reference ? p->reference : p->input; /* If the user has given a quantile range, then set the `greaterequal' and `lessthan' values. */ if( !isnan(p->quantmin) ) { /* If only one value was given, set the maximum quantile range. */ if( isnan(p->quantmax) ) p->quantmax = 1 - p->quantmin; /* Set the greater-equal value. */ tmp=gal_statistics_quantile(ref, p->quantmin, 1); tmp=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->greaterequal=*((float *)(tmp->array)); /* Set the lower-than value. */ tmp=gal_statistics_quantile(ref, p->quantmax, 1); tmp=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->lessthan=*((float *)(tmp->array)); } /* Set the condition. Note that the `greaterequal' name is for the data we want. So we will set the condition based on those that are less-than */ if(!isnan(p->greaterequal)) { tmp=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &one, NULL, 0, -1, NULL, NULL, NULL); *((float *)(tmp->array)) = p->greaterequal; cond_g=gal_arithmetic(GAL_ARITHMETIC_OP_LT, flags, ref, tmp); gal_data_free(tmp); } /* Same reasoning as above for `p->greaterthan'. */ if(!isnan(p->lessthan)) { tmp=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &one, NULL, 0, -1, NULL, NULL, NULL); *((float *)(tmp->array)) = p->lessthan; cond_l=gal_arithmetic(GAL_ARITHMETIC_OP_GE, flags, ref, tmp); gal_data_free(tmp); } /* Now, set the final condition. If both values were specified, then use the GAL_ARITHMETIC_OP_OR to merge them into one. */ switch( !isnan(p->greaterequal) + !isnan(p->lessthan) ) { case 0: return; /* No condition was specified, return. */ case 1: /* Only one condition was specified. */ cond = isnan(p->greaterequal) ? cond_l : cond_g; break; case 2: cond = gal_arithmetic(GAL_ARITHMETIC_OP_OR, flagsor, cond_l, cond_g); break; } /* Allocate a blank value to mask all pixels that don't satisfy the condition. */ blank=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &one, NULL, 0, -1, NULL, NULL, NULL); *((float *)(blank->array)) = NAN; /* Set all the pixels that satisfy the condition to blank. Note that a blank value will be used in the proper type of the input in the `where' operator.*/ gal_arithmetic(GAL_ARITHMETIC_OP_WHERE, flagsor, p->input, cond, blank); } /* Check if a sorted array is necessary and if so, then make a sorted array. */ static void ui_make_sorted_if_necessary(struct statisticsparams *p) { int is_necessary=0; gal_list_i32_t *tmp; /* Check in the one-row outputs. */ for(tmp=p->singlevalue; tmp!=NULL; tmp=tmp->next) switch(tmp->v) { case UI_KEY_MODE: case UI_KEY_MEDIAN: case UI_KEY_QUANTILE: case UI_KEY_QUANTFUNC: is_necessary=1; break; } /* Check in the rest of the outputs. */ if( is_necessary==0 && ( p->sigmaclip || !isnan(p->mirror) ) ) is_necessary=1; /* Do the sorting, we will keep the sorted array in a separate space, since the unsorted nature of the original dataset will help decrease floating point errors. If the input is already sorted, we'll just point it to the input.*/ if(is_necessary) { if( gal_statistics_is_sorted(p->input) ) p->sorted=p->input; else { p->sorted=gal_data_copy(p->input); gal_statistics_sort_increasing(p->sorted); } } } void ui_read_columns(struct statisticsparams *p) { int toomanycols=0; size_t size, counter=0; gal_data_t *cols, *tmp; gal_list_str_t *column=NULL; /* Define the columns that we want, note that they should be added to the list in reverse. */ if(p->refcol) gal_list_str_add(&column, p->refcol, 0); gal_list_str_add(&column, p->column, 0); /* Read the desired column(s). */ cols=gal_table_read(p->inputname, p->cp.hdu, column, p->cp.searchin, p->cp.ignorecase, p->cp.minmapsize, NULL); /* Put the columns into the proper gal_data_t. */ size=cols->size; while(cols!=NULL) { /* Pop out the top column. */ tmp=gal_list_data_pop(&cols); /* Make sure it has the proper size. */ if(tmp->size!=size) error(EXIT_FAILURE, 0, " read column number %zu has a %zu elements, " "while previous column(s) had %zu", counter, tmp->size, size); /* Make sure it is a usable datatype. */ switch(tmp->type) { case GAL_TYPE_BIT: case GAL_TYPE_STRLL: case GAL_TYPE_STRING: case GAL_TYPE_COMPLEX32: case GAL_TYPE_COMPLEX64: error(EXIT_FAILURE, 0, " read column number %zu has a %s type, " "which is not currently supported by %s", counter, gal_type_name(tmp->type, 1), PROGRAM_NAME); } /* Put the column into the proper pointer. */ switch(++counter) { case 1: p->input=tmp; break; case 2: if(p->refcol) p->reference=tmp; else toomanycols=1; break; default: toomanycols=1; } /* Print an error if there are too many columns: */ if(toomanycols) gal_tableintern_error_col_selection(p->inputname, p->cp.hdu, "too many " "columns were selected by the " "given values to the `--column' " "and/or `--refcol' options. Only " "one is acceptable for each."); } /* Clean up. */ gal_list_str_free(column, 0); } void ui_preparations(struct statisticsparams *p) { gal_data_t *check; struct gal_options_common_params *cp=&p->cp; struct gal_tile_two_layer_params *tl=&cp->tl; /* Read the input. */ if(p->isfits && p->hdu_type==IMAGE_HDU) { p->inputformat=INPUT_FORMAT_IMAGE; p->input=gal_fits_img_read(p->inputname, cp->hdu, cp->minmapsize, 0, 0); } else { ui_read_columns(p); p->inputformat=INPUT_FORMAT_TABLE; } /* Read the convolution kernel if necessary. */ if(p->sky && p->kernelname) p->kernel=gal_fits_img_read_kernel(p->kernelname, p->khdu, cp->minmapsize); /* Tile and channel sanity checks and preparations. */ if(p->ontile || p->sky) { /* Check the tiles and make the tile structure. */ gal_tile_full_sanity_check(p->inputname, p->cp.hdu, p->input, tl); gal_tile_full_two_layers(p->input, tl); gal_tile_full_permutation(tl); /* Make the tile check image if requested. */ if(tl->checktiles) { tl->tilecheckname=gal_checkset_automatic_output(cp, p->inputname, "_tiled.fits"); check=gal_tile_block_check_tiles(tl->tiles); if(p->inputformat==INPUT_FORMAT_IMAGE) gal_fits_img_write(check, tl->tilecheckname, NULL, PROGRAM_NAME); else { gal_checkset_writable_remove(tl->tilecheckname, 0, cp->dontdelete); gal_table_write(check, NULL, cp->tableformat, tl->tilecheckname, "TABLE"); } gal_data_free(check); } /* Set the steps image name. */ if(p->sky && p->checksky) p->checkskyname=gal_checkset_automatic_output(cp, p->inputname, "_sky_steps.fits"); } /* Set the out-of-range values in the input to blank. */ ui_out_of_range_to_blank(p); /* If we are not to work on tiles, then re-order and change the input. */ if(p->ontile==0 && p->sky==0) { /* Only keep the elements we want. */ gal_blank_remove(p->input); p->input->flag &= ~GAL_DATA_FLAG_HASBLANK ; p->input->flag |= GAL_DATA_FLAG_BLANK_CH ; /* Make sure there is data remaining: */ if(p->input->size==0) error(EXIT_FAILURE, 0, "%s: no data, maybe the `--greaterequal' or " "`--lessthan' options need to be adjusted", gal_fits_name_save_as_string(p->inputname, cp->hdu) ); /* Make the sorted array if necessary. */ ui_make_sorted_if_necessary(p); /* Set the number of output files. */ if( !isnan(p->mirror) ) ++p->numoutfiles; if( p->histogram || p->cumulative ) ++p->numoutfiles; } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct statisticsparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct statisticsparams *p) { /* Free the allocated arrays: */ free(p->cp.hdu); free(p->cp.output); gal_data_free(p->input); gal_data_free(p->reference); gal_list_f64_free(p->tp_args); gal_list_i32_free(p->singlevalue); gal_tile_full_free_contents(&p->cp.tl); if(p->sorted!=p->input) gal_data_free(p->sorted); } ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/main.c������������������������������������������������������������������0000644�0001750�0001750�00000003035�13121462410�014166� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Statistics - Statistical analysis on input dataset. Statistics is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "statistics.h" int main (int argc, char *argv[]) { struct timeval t1; struct statisticsparams p={{{0},0},0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ statistics(&p); /* Free all non-freed allocations. */ ui_free_report(&p); /* Return successfully.*/ return 0; } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/Makefile.in�������������������������������������������������������������0000644�0001750�0001750�00000211601�13217217706�015157� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; \ elif test -n '$(MAKE_HOST)'; then \ true; \ elif test -n '$(MAKE_VERSION)' && test -n '$(CURDIR)'; then \ true; \ else \ false; \ fi; \ } am__make_running_with_option = \ case $${target_option-} in \ ?) ;; \ *) echo "am__make_running_with_option: internal error: invalid" \ "target option '$${target_option-}' specified" >&2; \ exit 1;; \ esac; \ 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GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Statistics. # Statistics is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ aststatistics --help # Full list of options, short doc. # $ aststatistics -P # Print all options and used values. # $ info aststatistics # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Input image: # Sky and its STD settings khdu 1 modmedqdiff 0.01 smoothwidth 3 sclipparams 3,0.1 # Histogram and CFP settings numasciibins 70 asciiheight 10 numbins 100 mirrordist 1.5 �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/statistics/Makefile.am�������������������������������������������������������������0000644�0001750�0001750�00000002632�13121462410�015134� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = aststatistics aststatistics_LDADD = -lgnuastro aststatistics_SOURCES = main.c ui.c sky.c statistics.c EXTRA_DIST = main.h authors-cite.h args.h ui.h sky.h statistics.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = aststatistics.conf ������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/�����������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220467�013302� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/threshold.h������������������������������������������������������������0000644�0001750�0001750�00000003272�13156610402�015365� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef THRESHOLD_H #define THRESHOLD_H #define THRESHOLD_NO_ERODE_VALUE 2 enum threshold_type { THRESHOLD_QUANTILES, THRESHOLD_SKY_STD, }; void threshold_apply(struct noisechiselparams *p, float *value1, float *value2, int type); void threshold_write_sn_table(struct noisechiselparams *p, gal_data_t *sntable, gal_data_t *snind, char *filename, gal_list_str_t *comments); void threshold_interp_smooth(struct noisechiselparams *p, gal_data_t **first, gal_data_t **second, gal_data_t **third, char *filename); void threshold_quantile_find_apply(struct noisechiselparams *p); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/sky.h������������������������������������������������������������������0000644�0001750�0001750�00000002203�13121462410�014164� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef SKY_H #define SKY_H void sky_and_std(struct noisechiselparams *p, char *checkname); void sky_subtract(struct noisechiselparams *p); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/segmentation.h���������������������������������������������������������0000644�0001750�0001750�00000002124�13121462410�016055� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef SEGMENTATION_H #define SEGMENTATION_H void segmentation(struct noisechiselparams *p); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/noisechisel.h����������������������������������������������������������0000644�0001750�0001750�00000002121�13121462410�015662� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef NOISECHISEL_H #define NOISECHISEL_H void noisechisel(struct noisechiselparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/detection.h������������������������������������������������������������0000644�0001750�0001750�00000002201�13121462410�015332� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef DETECTION_H #define DETECTION_H void detection_initial(struct noisechiselparams *p); void detection(struct noisechiselparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/clumps.h���������������������������������������������������������������0000644�0001750�0001750�00000007177�13176441456�014721� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef CLUMPS_H #define CLUMPS_H /* Constants for the clump over-segmentation. */ #define CLUMPS_INIT -1 #define CLUMPS_RIVER -2 #define CLUMPS_TMPCHECK -3 /* Parameters for all threads. */ struct clumps_params { /* General */ int step; /* Counter if we want to check steps. */ int sky0_det1; /* If working on the Sky or Detections. */ struct noisechiselparams *p; /* Pointer to main NoiseChisel parameters. */ pthread_mutex_t labmutex; /* Mutex to change the total numbers. */ /* For Sky region. */ gal_data_t *sn; /* Array of clump S/N tables. */ gal_data_t *snind; /* Array of clump S/N index (for check). */ /* For detections. */ gal_data_t *labindexs; /* Array of `gal_data_t' with obj indexs. */ size_t totobjects; /* Total number of objects at any point. */ size_t totclumps; /* Total number of clumps at any point. */ }; /* Parameters for one thread (a tile or a detected region). */ struct clumps_thread_params { size_t id; /* ID of this detection/tile over tile. */ size_t *topinds; /* Indexs of all local maxima. */ size_t numinitclumps; /* Number of clumps in tile/detection. */ size_t numtrueclumps; /* Number of true clumps in tile/detection.*/ size_t numobjects; /* Number of objects over this clump. */ float std; /* Standard deviation of noise on center. */ gal_data_t *indexs; /* Array containing indexs of this det. */ gal_data_t *diffuseindexs; /* Diffuse region (after finding clumps). */ gal_data_t *info; /* Information for all clumps. */ gal_data_t *sn; /* Signal-to-noise ratio for these clumps. */ gal_data_t *snind; /* Index of S/N for these clumps. */ gal_data_t *clumptoobj; /* Index of object that a clump belongs to.*/ struct clumps_params *clprm; /* Pointer to main structure. */ }; void clumps_oversegment(struct clumps_thread_params *cltprm); void clumps_grow_prepare_initial(struct clumps_thread_params *cltprm); void clumps_grow_prepare_final(struct clumps_thread_params *cltprm); void clumps_grow(gal_data_t *labels, gal_data_t *diffuseindexs, int withrivers, int connectivity); void clumps_true_find_sn_thresh(struct noisechiselparams *p); void clumps_make_sn_table(struct clumps_thread_params *cltprm); gal_data_t * clumps_det_label_indexs(struct noisechiselparams *p); void clumps_det_keep_true_relabel(struct clumps_thread_params *cltprm); #endif �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/ui.h�������������������������������������������������������������������0000644�0001750�0001750�00000006035�13177434204�014015� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_DETECTION = GAL_OPTIONS_GROUP_AFTER_COMMON, UI_GROUP_SEGMENTATION, }; /* Available letters for short options: a b f j l n u x z A H J W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_LARGETILESIZE = 'L', UI_KEY_KERNEL = 'k', UI_KEY_WIDEKERNEL = 'w', UI_KEY_SKYSUBTRACTED = 'E', UI_KEY_MINSKYFRAC = 'B', UI_KEY_MIRRORDIST = 'r', UI_KEY_MODMEDQDIFF = 'Q', UI_KEY_QTHRESH = 't', UI_KEY_ERODE = 'e', UI_KEY_OPENING = 'p', UI_KEY_SIGMACLIP = 's', UI_KEY_DTHRESH = 'R', UI_KEY_DETSNMINAREA = 'i', UI_KEY_DETQUANT = 'c', UI_KEY_DETGROWQUANT = 'd', UI_KEY_SEGSNMINAREA = 'm', UI_KEY_SEGQUANT = 'g', UI_KEY_KEEPMAXNEARRIVER = 'v', UI_KEY_GTHRESH = 'G', UI_KEY_MINRIVERLENGTH = 'y', UI_KEY_OBJBORDERSN = 'O', UI_KEY_CONTINUEAFTERCHECK = 'C', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_KHDU = 1000, UI_KEY_CONVOLVED, UI_KEY_CONVOLVEDHDU, UI_KEY_WKHDU, UI_KEY_MINNUMFALSE, UI_KEY_ONLYDETECTION, UI_KEY_GROWNCLUMPS, UI_KEY_SMOOTHWIDTH, UI_KEY_QTHRESHTILEQUANT, UI_KEY_CHECKQTHRESH, UI_KEY_ERODENGB, UI_KEY_NOERODEQUANT, UI_KEY_OPENINGNGB, UI_KEY_CHECKDETSKY, UI_KEY_CHECKDETSN, UI_KEY_DETGROWMAXHOLESIZE, UI_KEY_CLEANGROWNDET, UI_KEY_CHECKDETECTION, UI_KEY_CHECKSKY, UI_KEY_CHECKCLUMPSN, UI_KEY_CHECKSEGMENTATION, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct noisechiselparams *p); void ui_abort_after_check(struct noisechiselparams *p, char *filename, char *file2name, char *description); void ui_free_report(struct noisechiselparams *p, struct timeval *t1); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/args.h�����������������������������������������������������������������0000644�0001750�0001750�00000034601�13216276304�014333� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Options in argp_option format. */ struct argp_option program_options[] = { /* Input options. */ { "kernel", UI_KEY_KERNEL, "STR", 0, "Filename of kernel to convolve with input", GAL_OPTIONS_GROUP_INPUT, &p->kernelname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "khdu", UI_KEY_KHDU, "STR", 0, "HDU containing kernel image.", GAL_OPTIONS_GROUP_INPUT, &p->khdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "convolved", UI_KEY_CONVOLVED, "STR", 0, "Convolved image file to avoid convolution.", GAL_OPTIONS_GROUP_INPUT, &p->convolvedname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "convolvedhdu", UI_KEY_CONVOLVEDHDU, "STR", 0, "HDU/extension of convolved image in file.", GAL_OPTIONS_GROUP_INPUT, &p->convolvedhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "widekernel", UI_KEY_WIDEKERNEL, "STR", 0, "Filename of wider kernel for better qthresh", GAL_OPTIONS_GROUP_INPUT, &p->widekernelname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "wkhdu", UI_KEY_WKHDU, "STR", 0, "HDU containing wide kernel image.", GAL_OPTIONS_GROUP_INPUT, &p->wkhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "skysubtracted", UI_KEY_SKYSUBTRACTED, 0, 0, "Input is Sky subtracted (for error estimation).", GAL_OPTIONS_GROUP_INPUT, &p->skysubtracted, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "minskyfrac", UI_KEY_MINSKYFRAC, "FLT", 0, "Min. fraction of undetected area in tile.", GAL_OPTIONS_GROUP_INPUT, &p->minskyfrac, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "minnumfalse", UI_KEY_MINNUMFALSE, "INT", 0, "Minimum number for S/N estimation.", GAL_OPTIONS_GROUP_INPUT, &p->minnumfalse, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Tessellation. */ { "largetilesize", UI_KEY_LARGETILESIZE, "INT[,INT]", 0, "Sim. to --tilesize, but for larger tiles.", GAL_OPTIONS_GROUP_TESSELLATION, &p->ltl.tilesize, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_sizes_reverse }, /* Output options. */ { "onlydetection", UI_KEY_ONLYDETECTION, 0, 0, "Stop at the end of detection.", GAL_OPTIONS_GROUP_OUTPUT, &p->onlydetection, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Detection. */ { 0, 0, 0, 0, "Detection:", UI_GROUP_DETECTION }, { "mirrordist", UI_KEY_MIRRORDIST, "FLT", 0, "Max. dist. (error multip.) to find mode.", UI_GROUP_DETECTION, &p->mirrordist, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "modmedqdiff", UI_KEY_MODMEDQDIFF, "FLT", 0, "Max. mode and median quant diff. per tile.", UI_GROUP_DETECTION, &p->modmedqdiff, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "qthresh", UI_KEY_QTHRESH, "FLT", 0, "Quantile threshold on convolved image.", UI_GROUP_DETECTION, &p->qthresh, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LT_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "qthreshtilequant", UI_KEY_QTHRESHTILEQUANT, "FLT", 0, "Remove tiles at higher quantiles.", UI_GROUP_DETECTION, &p->qthreshtilequant, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "smoothwidth", UI_KEY_SMOOTHWIDTH, "INT", 0, "Flat kernel width to smooth interpolated.", UI_GROUP_DETECTION, &p->smoothwidth, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_0_OR_ODD, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checkqthresh", UI_KEY_CHECKQTHRESH, 0, 0, "Save quantile threshold estimation in file.", UI_GROUP_DETECTION, &p->checkqthresh, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "erode", UI_KEY_ERODE, "INT", 0, "Number of erosions after thresholding.", UI_GROUP_DETECTION, &p->erode, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "erodengb", UI_KEY_ERODENGB, "INT", 0, "4 or 8 connectivity in erosion.", UI_GROUP_DETECTION, &p->erodengb, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "noerodequant", UI_KEY_NOERODEQUANT, "FLT", 0, "Quantile for no erosion.", UI_GROUP_DETECTION, &p->noerodequant, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "opening", UI_KEY_OPENING, "INT", 0, "Depth of opening after erosion.", UI_GROUP_DETECTION, &p->opening, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "openingngb", UI_KEY_OPENINGNGB, "INT", 0, "4 or 8 connectivity in opening.", UI_GROUP_DETECTION, &p->openingngb, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "sigmaclip", UI_KEY_SIGMACLIP, "FLT,FLT", 0, "Sigma multiple and, tolerance or number.", UI_GROUP_DETECTION, &p->sigmaclip, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_read_sigma_clip }, { "checkdetsky", UI_KEY_CHECKDETSKY, 0, 0, "Save Sky value estimation for pseudo-dets.", UI_GROUP_DETECTION, &p->checkdetsky, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "dthresh", UI_KEY_DTHRESH, "FLT", 0, "Sigma threshold for Pseudo-detections.", UI_GROUP_DETECTION, &p->dthresh, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "detsnminarea", UI_KEY_DETSNMINAREA, "INT", 0, "Min. pseudo-detection area for S/N dist.", UI_GROUP_DETECTION, &p->detsnminarea, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checkdetsn", UI_KEY_CHECKDETSN, 0, 0, "Save pseudo-detection S/N values to a file.", UI_GROUP_DETECTION, &p->checkdetsn, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "detquant", UI_KEY_DETQUANT, "FLT", 0, "Quantile in pseudo-det. to define true.", UI_GROUP_DETECTION, &p->detquant, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0_LT_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "detgrowquant", UI_KEY_DETGROWQUANT, "FLT", 0, "Minimum quant. to expand true detections.", UI_GROUP_DETECTION, &p->detgrowquant, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "detgrowmaxholesize", UI_KEY_DETGROWMAXHOLESIZE, "INT", 0, "Max. area of holes after growth to fill.", UI_GROUP_DETECTION, &p->detgrowmaxholesize, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "cleangrowndet", UI_KEY_CLEANGROWNDET, 0, 0, "Remove small S/N grown detections.", UI_GROUP_DETECTION, &p->cleangrowndet, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checkdetection", UI_KEY_CHECKDETECTION, 0, 0, "Save all the detection steps to a file.", UI_GROUP_DETECTION, &p->checkdetection, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checksky", UI_KEY_CHECKSKY, 0, 0, "Final sky and its STD steps in a file.", UI_GROUP_DETECTION, &p->checksky, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Segmentation */ { 0, 0, 0, 0, "Segmentation:", UI_GROUP_SEGMENTATION }, { "segsnminarea", UI_KEY_SEGSNMINAREA, "INT", 0, "Minimum area of clumps for S/N estimation.", UI_GROUP_SEGMENTATION, &p->segsnminarea, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checkclumpsn", UI_KEY_CHECKCLUMPSN, 0, 0, "Save Sky clump S/N values into a file.", UI_GROUP_SEGMENTATION, &p->checkclumpsn, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "segquant", UI_KEY_SEGQUANT, "FLT", 0, "S/N Quantile of true sky clumps.", UI_GROUP_SEGMENTATION, &p->segquant, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "keepmaxnearriver", UI_KEY_KEEPMAXNEARRIVER, 0, 0, "Keep clumps with peak touching a river.", UI_GROUP_SEGMENTATION, &p->keepmaxnearriver, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "gthresh", UI_KEY_GTHRESH, "FLT", 0, "Multiple of STD to stop growing clumps.", UI_GROUP_SEGMENTATION, &p->gthresh, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "minriverlength", UI_KEY_MINRIVERLENGTH, "INT", 0, "Minimum len of useful grown clump rivers.", UI_GROUP_SEGMENTATION, &p->minriverlength, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "objbordersn", UI_KEY_OBJBORDERSN, "FLT", 0, "Min. S/N for grown clumps as one object.", UI_GROUP_SEGMENTATION, &p->objbordersn, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "grownclumps", UI_KEY_GROWNCLUMPS, 0, 0, "Save grown clumps instead of original.", UI_GROUP_SEGMENTATION, &p->grownclumps, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "checksegmentation", UI_KEY_CHECKSEGMENTATION, 0, 0, "Store segmentation steps in a file.", UI_GROUP_SEGMENTATION, &p->checksegmentation, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Operating mode options. */ { "continueaftercheck", UI_KEY_CONTINUEAFTERCHECK, 0, 0, "Continue processing after checks.", GAL_OPTIONS_GROUP_OPERATING_MODE, &p->continueaftercheck, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* End of options. */ {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif �������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/authors-cite.h���������������������������������������������������������0000644�0001750�0001750�00000003004�13211076737�016002� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/main.h�����������������������������������������������������������������0000644�0001750�0001750�00000017103�13177434204�014322� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "NoiseChisel" /* Program full name. */ #define PROGRAM_EXEC "astnoisechisel" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Main program parameters structure */ struct noisechiselparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ struct gal_tile_two_layer_params ltl;/* Large tessellation. */ char *inputname; /* Input filename. */ char *kernelname; /* Input kernel filename. */ char *widekernelname; /* Name of wider kernel to be used. */ char *convolvedname; /* Convolved image (to avoid convolution).*/ char *convolvedhdu; /* HDU of convolved image. */ char *khdu; /* Kernel HDU. */ char *wkhdu; /* Wide kernel HDU. */ uint8_t skysubtracted; /* Input has been Sky subtracted before. */ float minskyfrac; /* Undetected area min. frac. in tile. */ size_t minnumfalse; /* Min No. of det/seg for true quantile. */ uint8_t onlydetection; /* Do not do any segmentation. */ uint8_t grownclumps; /* Save grown clumps instead of original. */ uint8_t continueaftercheck; /* Don't abort after the check steps. */ float mirrordist; /* Maximum distance to check mode sym. */ float modmedqdiff; /* Difference between mode and median. */ float qthresh; /* Quantile threshold on convolved image. */ float qthreshtilequant; /* Remove tiles with lower quantile. */ size_t smoothwidth; /* Width of flat kernel to smooth. */ uint8_t checkqthresh; /* Save the quantile threhsold steps. */ size_t erode; /* Number of erosions after thresholding. */ size_t erodengb; /* Connectivity for erosion. */ float noerodequant; /* Quantile for no erosion. */ size_t opening; /* Depth of opening after erosion. */ size_t openingngb; /* Connectivity to use for opening. */ double sigmaclip[2]; /* Sigma-clipping parameters. */ uint8_t checkdetsky; /* Check pseudo-detection sky value. */ float dthresh; /* Sigma threshold for Pseudo-detections. */ size_t detsnminarea; /* Minimum pseudo-detection area for S/N. */ uint8_t checkdetsn; /* Save pseudo-detection S/N values. */ float detquant; /* True detection quantile. */ float detgrowquant; /* Quantile to grow true detections. */ size_t detgrowmaxholesize; /* Max. size of holes to fill in growth. */ uint8_t cleangrowndet; /* Remove grown objects with small S/N. */ uint8_t checkdetection; /* Save all detection steps to a file. */ uint8_t checksky; /* Check the Sky value estimation. */ size_t segsnminarea; /* Minimum area for segmentation. */ uint8_t checkclumpsn; /* Save the clump S/N values to a file. */ float segquant; /* Quantile of clumps in sky for true S/N.*/ uint8_t keepmaxnearriver; /* Keep clumps with a peak near a river. */ float gthresh; /* Multiple of STD to stop growing clumps.*/ size_t minriverlength; /* Min, len of good grown clump rivers. */ float objbordersn; /* Minimum S/N for grown clumps to be one.*/ uint8_t checksegmentation; /* Save the segmentation steps in file. */ /* Internal. */ char *qthreshname; /* Name of Quantile threshold check image.*/ char *detskyname; /* Name of Initial det sky check image. */ char *detsn_s_name; /* Sky pseudo-detections S/N name. */ char *detsn_d_name; /* Detection pseudo-detections S/N name. */ char *detsn_D_name; /* Final detection S/N name. */ char *detectionname; /* Name of detection steps file. */ char *skyname; /* Name of Sky estimation steps file. */ char *clumpsn_s_name; /* Sky clump S/N name. */ char *clumpsn_d_name; /* Detection clumps S/N name. */ char *segmentationname; /* Name of segmentation steps file. */ gal_data_t *input; /* Input image. */ gal_data_t *kernel; /* Sharper kernel. */ gal_data_t *widekernel; /* Wider kernel. */ gal_data_t *conv; /* Convolved wth sharper kernel. */ gal_data_t *wconv; /* Convolved with wider kernel. */ gal_data_t *binary; /* For binary operations. */ gal_data_t *olabel; /* Labels of objects in the detection. */ gal_data_t *clabel; /* Labels of clumps in the detection. */ gal_data_t *expand_thresh; /* Quantile threshold to expand per tile. */ gal_data_t *sky; /* Mean of undetected pixels, per tile. */ gal_data_t *std; /* STD of undetected pixels, per tile. */ size_t maxtcontig; /* Maximum contiguous space for a tile. */ size_t maxltcontig; /* Maximum contiguous space for a tile. */ size_t *maxtsize; /* Maximum size of a single small tile. */ size_t *maxltsize; /* Maximum size of a single large tile. */ time_t rawtime; /* Starting time of the program. */ float medstd; /* Median STD before interpolation. */ float minstd; /* Minimum STD before interpolation. */ float maxstd; /* Maximum STD before interpolation. */ float cpscorr; /* Counts/second correction. */ size_t numinitialdets; /* Number of initial detections. */ size_t numdetections; /* Number of final detections. */ size_t numclumps; /* Number of true clumps. */ size_t numobjects; /* Number of objects. */ float detsnthresh; /* Pseudo-detection S/N threshold. */ float clumpsnthresh; /* Clump S/N threshold. */ }; #endif �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/threshold.c������������������������������������������������������������0000644�0001750�0001750�00000061147�13216276304�015373� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/threads.h> #include <gnuastro/statistics.h> #include <gnuastro/interpolate.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "ui.h" #include "threshold.h" /**********************************************************************/ /*************** Apply a given threshold. *****************/ /**********************************************************************/ struct threshold_apply_p { float *value1; float *value2; int kind; struct noisechiselparams *p; }; /* Apply the threshold on the tiles given to this thread. */ static void * threshold_apply_on_thread(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct threshold_apply_p *taprm=(struct threshold_apply_p *)(tprm->params); struct noisechiselparams *p=taprm->p; size_t i, tid; void *tarray=NULL; gal_data_t *tile, *tblock=NULL; float *value1=taprm->value1, *value2=taprm->value2; /* Go over all the tiles assigned to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* For easy reading. */ tid=tprm->indexs[i]; tile=&p->cp.tl.tiles[tid]; /* Based on the kind of threshold. */ switch(taprm->kind) { /* This is a quantile threshold. */ case THRESHOLD_QUANTILES: /* Correct the tile's pointers to apply the threshold on the convolved image. */ if(p->conv) { tarray=tile->array; tblock=tile->block; tile->array=gal_tile_block_relative_to_other(tile, p->conv); tile->block=p->conv; } /* Apply the threshold: When the `>' comparison fails, it can be either because the pixel was actually smaller than the threshold, or that it was a NaN value. In the first case, return 0, in the second, return a blank value. We already know if a tile contains a blank value (which is a constant over the whole loop). So before checking if the value is blank, see if the tile actually has a blank value. This will help in efficiency, because the compiler can move this check out of the loop and only check for NaN values when we know the tile has blank pixels. */ GAL_TILE_PO_OISET(float, uint8_t, tile, p->binary, 1, 0, { *o = ( *i > value1[tid] ? ( *i > value2[tid] ? THRESHOLD_NO_ERODE_VALUE : 1 ) : ( (tile->flag & GAL_DATA_FLAG_HASBLANK) && !(*i==*i) ? GAL_BLANK_UINT8 : 0 ) ); }); /* Revert the tile's pointers back to what they were. */ if(p->conv) { tile->array=tarray; tile->block=tblock; } break; /* This is a Sky and Sky STD threshold. */ case THRESHOLD_SKY_STD: /* See the explanation above the same step in the quantile threshold for an explanation. */ GAL_TILE_PO_OISET(float, uint8_t, tile, p->binary, 1, 0, { *o = ( ( *i - value1[tid] > p->dthresh * value2[tid] ) ? 1 : ( (tile->flag & GAL_DATA_FLAG_HASBLANK) && !(*i==*i) ? GAL_BLANK_UINT8 : 0 ) ); }); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we " "can address the problem. A value of %d had for " "`taprm->kind' is not valid", __func__, PACKAGE_BUGREPORT, taprm->kind); } } /* Wait until all the other threads finish. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* Apply a given threshold threshold on the tiles. */ void threshold_apply(struct noisechiselparams *p, float *value1, float *value2, int kind) { struct threshold_apply_p taprm={value1, value2, kind, p}; gal_threads_spin_off(threshold_apply_on_thread, &taprm, p->cp.tl.tottiles, p->cp.numthreads); } /**********************************************************************/ /*************** Write S/N values *****************/ /**********************************************************************/ void threshold_write_sn_table(struct noisechiselparams *p, gal_data_t *insn, gal_data_t *inind, char *filename, gal_list_str_t *comments) { gal_data_t *sn, *ind, *cols; /* Remove all blank elements. The index and sn values must have the same set of blank elements, but checking on the integer array is faster. */ if( gal_blank_present(inind, 1) ) { ind=gal_data_copy(inind); sn=gal_data_copy(insn); gal_blank_remove(ind); gal_blank_remove(sn); } else { sn = insn; ind = inind; } /* Set the columns. */ cols = ind; cols->next = sn; /* Prepare the comments. */ gal_table_comments_add_intro(&comments, PROGRAM_STRING, &p->rawtime); /* write the table. */ gal_checkset_writable_remove(filename, 0, 1); gal_table_write(cols, comments, p->cp.tableformat, filename, "SN"); /* Clean up (if necessary). */ if(sn!=insn) gal_data_free(sn); if(ind==inind) ind->next=NULL; else gal_data_free(ind); } /**********************************************************************/ /*************** Interpolation and smoothing *****************/ /**********************************************************************/ /* Interpolate and smooth the values for each tile over the whole image. */ void threshold_interp_smooth(struct noisechiselparams *p, gal_data_t **first, gal_data_t **second, gal_data_t **third, char *filename) { gal_data_t *tmp; struct gal_options_common_params *cp=&p->cp; struct gal_tile_two_layer_params *tl=&cp->tl; /* A small sanity check. */ if( (*first)->next ) error(EXIT_FAILURE, 0, "%s: `first' must not have any `next' pointer.", __func__); if( (*second)->next ) error(EXIT_FAILURE, 0, "%s: `second' must not have any `next' pointer.", __func__); if( third && (*third)->next ) error(EXIT_FAILURE, 0, "%s: `third' must not have any `next' pointer.", __func__); /* Do the interpolation of both arrays. */ (*first)->next = *second; if(third) (*second)->next = *third; tmp=gal_interpolate_close_neighbors(*first, tl, cp->interpnumngb, cp->numthreads, cp->interponlyblank, 1); gal_data_free(*first); gal_data_free(*second); if(third) gal_data_free(*third); *first=tmp; *second=(*first)->next; if(third) { *third=(*second)->next; (*third)->next=NULL; } (*first)->next=(*second)->next=NULL; if(filename) { (*first)->name="THRESH1_INTERP"; (*second)->name="THRESH2_INTERP"; if(third) (*third)->name="THRESH3_INTERP"; gal_tile_full_values_write(*first, tl, 1, filename, NULL, PROGRAM_NAME); gal_tile_full_values_write(*second, tl, 1, filename, NULL, PROGRAM_NAME); if(third) gal_tile_full_values_write(*third, tl, 1, filename, NULL, PROGRAM_NAME); (*first)->name = (*second)->name = NULL; if(third) (*third)->name=NULL; } /* Smooth the threshold if requested. */ if(p->smoothwidth>1) { /* Smooth the first. */ tmp=gal_tile_full_values_smooth(*first, tl, p->smoothwidth, p->cp.numthreads); gal_data_free(*first); *first=tmp; /* Smooth the second */ tmp=gal_tile_full_values_smooth(*second, tl, p->smoothwidth, p->cp.numthreads); gal_data_free(*second); *second=tmp; /* Smooth the third */ if(third) { tmp=gal_tile_full_values_smooth(*third, tl, p->smoothwidth, p->cp.numthreads); gal_data_free(*third); *third=tmp; } /* Add them to the check image. */ if(filename) { (*first)->name="THRESH1_SMOOTH"; (*second)->name="THRESH2_SMOOTH"; if(third) (*third)->name="THRESH3_SMOOTH"; gal_tile_full_values_write(*first, tl, 1, filename, NULL, PROGRAM_NAME); gal_tile_full_values_write(*second, tl, 1, filename, NULL, PROGRAM_NAME); if(third) gal_tile_full_values_write(*third, tl, 1, filename, NULL, PROGRAM_NAME); (*first)->name = (*second)->name = NULL; if(third) (*third)->name=NULL; } } } /**************************************************************** ************ Quantile threshold ************ ****************************************************************/ struct qthreshparams { gal_data_t *erode_th; gal_data_t *noerode_th; gal_data_t *expand_th; void *usage; struct noisechiselparams *p; }; static void * qthresh_on_tile(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct qthreshparams *qprm=(struct qthreshparams *)tprm->params; struct noisechiselparams *p=qprm->p; double *darr; void *tarray=NULL; int type=qprm->erode_th->type; gal_data_t *modeconv = p->wconv ? p->wconv : p->conv; gal_data_t *tile, *mode, *qvalue, *usage, *tblock=NULL; size_t i, tind, twidth=gal_type_sizeof(type), ndim=p->input->ndim; /* Put the temporary usage space for this thread into a data set for easy processing. */ usage=gal_data_alloc(gal_data_ptr_increment(qprm->usage, tprm->id*p->maxtcontig, type), type, ndim, p->maxtsize, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Go over all the tiles given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* Re-initialize the usage array's space (will be changed in `gal_data_copy_to_allocated' for each tile). */ usage->ndim=ndim; usage->size=p->maxtcontig; memcpy(usage->dsize, p->maxtsize, ndim*sizeof *p->maxtsize); /* For easy reading. */ tind = tprm->indexs[i]; tile = &p->cp.tl.tiles[tind]; /* Temporarily change the tile's pointers so we can do the work on the convolved image, then copy the desired contents into the already allocated `usage' array. */ tarray=tile->array; tblock=tile->block; tile->array=gal_tile_block_relative_to_other(tile, modeconv); tile->block=modeconv; gal_data_copy_to_allocated(tile, usage); tile->array=tarray; tile->block=tblock; /* Find the mode on this tile, note that we have set the `inplace' flag to `1' to avoid extra allocation. */ mode=gal_statistics_mode(usage, p->mirrordist, 1); /* Check the mode value. Note that if the mode is not accurate, then the contents of `darr' will be NaN and all conditions will fail. In such cases, the tile will be ignored. */ darr=mode->array; if( fabs(darr[1]-0.5f) < p->modmedqdiff ) { /* The mode was found on the wider convolved image, but the qthresh values have to be found on the sharper convolved images. This is because the distribution becomes more skewed with a wider kernel, helping us find tiles with no data more easily. But for the quantile threshold, we want to use the sharper convolved image to loose less of the spatial information. */ if(modeconv!=p->conv) { tarray=tile->array; tblock=tile->block; tile->array=gal_tile_block_relative_to_other(tile, p->conv); tile->block=p->conv; usage->ndim=ndim; /* Since usage was modified in */ usage->size=p->maxtcontig; /* place, it needs to be */ gal_data_copy_to_allocated(tile, usage); /* re-initialized. */ tile->array=tarray; tile->block=tblock; } /* Get the erosion quantile for this tile and save it. Note that the type of `qvalue' is the same as the input dataset. */ qvalue=gal_statistics_quantile(usage, p->qthresh, 1); memcpy(gal_data_ptr_increment(qprm->erode_th->array, tind, type), qvalue->array, twidth); gal_data_free(qvalue); /* Same for the no-erode quantile. */ qvalue=gal_statistics_quantile(usage, p->noerodequant, 1); memcpy(gal_data_ptr_increment(qprm->noerode_th->array, tind, type), qvalue->array, twidth); gal_data_free(qvalue); /* Same for the expansion quantile. */ if(p->detgrowquant!=1.0f) { qvalue=gal_statistics_quantile(usage, p->detgrowquant, 1); memcpy(gal_data_ptr_increment(qprm->expand_th->array, tind, type), qvalue->array, twidth); gal_data_free(qvalue); } } else { gal_blank_write(gal_data_ptr_increment(qprm->erode_th->array, tind, type), type); gal_blank_write(gal_data_ptr_increment(qprm->noerode_th->array, tind, type), type); if(p->detgrowquant!=1.0f) gal_blank_write(gal_data_ptr_increment(qprm->expand_th->array, tind, type), type); } /* Clean up and fix the tile's pointers. */ gal_data_free(mode); } /* Clean up and wait for the other threads to finish, then return. */ usage->array=NULL; /* Not allocated here. */ gal_data_free(usage); if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* The main working function for `threshold_qthresh_clean'. The main purpose/problem is this: when we have channels, the qthresh values for each channel should be treated independently. */ static void threshold_qthresh_clean_work(struct noisechiselparams *p, gal_data_t *first, gal_data_t *second, gal_data_t *third, size_t start, size_t number) { gal_data_t *quantile; size_t i, osize=first->size; float *oa1=NULL, *oa2=NULL, *oa3=NULL; float q, *arr1=NULL, *arr2=NULL, *arr3=NULL; /* A small sanity check. */ if(first->type!=GAL_TYPE_FLOAT32) error(EXIT_FAILURE, 0, "%s: datatype has to be float32", __func__); /* Correct the arrays (if necessary). IMPORTANT: The datasets are multi-dimensional. However, when estimating the quantile, their dimensionality doesn't matter (only the `size' element is checked by `gal_statistics_quantile', not `ndim' or `dsize'). So we just need to correct `size' if channels are to be considered. */ if(start || number!=first->size) { /* Keep the original values for re-setting later. */ oa1=first->array; oa2=second->array; if(third) oa3=third->array; /* Increment the array pointers. */ first->array=gal_data_ptr_increment(first->array, start, first->type); second->array=gal_data_ptr_increment(second->array, start, second->type); if(third) third->array=gal_data_ptr_increment(third->array, start, third->type); /* Correct their sizes. */ first->size=number; second->size=number; if(third) third->size=number; } /* Find the quantile and remove all tiles that are more than it in the first array. */ arr1=first->array; quantile=gal_statistics_quantile(first, p->qthreshtilequant, 0); q=*((float *)(quantile->array)); for(i=0;i<first->size;++i) /* Just note that we have blank (NaN) values, so to avoid doing a NaN check with `isnan', we will check if the value is below the quantile, if it succeeds (isn't NaN and is below the quantile), then we'll put it's actual value, otherwise, a NaN. */ arr1[i] = arr1[i]<q ? arr1[i] : NAN; gal_data_free(quantile); /* Second quantile threshold. */ arr2=second->array; quantile=gal_statistics_quantile(second, p->qthreshtilequant, 0); q=*((float *)(quantile->array)); for(i=0;i<second->size;++i) arr2[i] = arr2[i]<q ? arr2[i] : NAN; gal_data_free(quantile); /* The third (if it exists). */ if(third) { arr3=third->array; quantile=gal_statistics_quantile(third, p->qthreshtilequant, 0); q=*((float *)(quantile->array)); for(i=0;i<third->size;++i) arr3[i] = arr3[i]<q ? arr3[i] : NAN; gal_data_free(quantile); } /* Make sure all three have the same NaN pixels. */ for(i=0;i<first->size;++i) if( isnan(arr1[i]) || isnan(arr2[i]) || isnan(arr3[i]) ) { arr1[i] = arr2[i] = NAN; if(third) arr3[i] = NAN; } /* Correct the values if they were changed. */ if(start || number!=osize) { first->array=oa1; second->array=oa2; first->size = second->size = osize; if(third) { third->array=oa3; third->size=osize; } } } /* Clean higher valued quantile thresholds: useful when the diffuse (almost flat) structures are much larger than the tile size. */ static void threshold_qthresh_clean(struct noisechiselparams *p, gal_data_t *first, gal_data_t *second, gal_data_t *third, char *filename) { size_t i; struct gal_tile_two_layer_params *tl=&p->cp.tl; /* A small sanity check: */ if(first->size!=tl->tottiles) error(EXIT_FAILURE, 0, "%s: `first->size' and `tl->tottiles' must have " "the same value, but they don't: %zu, %zu", __func__, first->size, tl->tottiles); /* If the input is from a tile structure and the user has asked to ignore channels, then re-order the values. */ for(i=0;i<tl->totchannels;++i) threshold_qthresh_clean_work(p, first, second, third, i*tl->tottilesinch, tl->tottilesinch); /* If the user wants to see the steps. */ if(p->qthreshname) { first->name="QTHRESH_ERODE_CLEAN"; second->name="QTHRESH_NOERODE_CLEAN"; gal_tile_full_values_write(first, tl, 1, p->qthreshname, NULL, PROGRAM_NAME); gal_tile_full_values_write(second, tl, 1, p->qthreshname, NULL, PROGRAM_NAME); first->name=second->name=NULL; if(third) { third->name="QTHRESH_EXPAND_CLEAN"; gal_tile_full_values_write(third, tl, 1, p->qthreshname, NULL, PROGRAM_NAME); third->name=NULL; } } } void threshold_quantile_find_apply(struct noisechiselparams *p) { char *msg; struct timeval t1; struct qthreshparams qprm; struct gal_options_common_params *cp=&p->cp; struct gal_tile_two_layer_params *tl=&cp->tl; /* Get the starting time if necessary. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); /* Add image to check image if requested. If the user has asked for `oneelempertile', then the size of values is not going to be the same as the input, making it hard to inspect visually. So we'll only put the full input when `oneelempertile' isn't requested. */ if(p->qthreshname && !tl->oneelempertile) { gal_fits_img_write(p->conv ? p->conv : p->input, p->qthreshname, NULL, PROGRAM_NAME); if(p->wconv) gal_fits_img_write(p->wconv ? p->wconv : p->input, p->qthreshname, NULL, PROGRAM_NAME); } /* Allocate space for the quantile threshold values. */ qprm.erode_th=gal_data_alloc(NULL, p->input->type, p->input->ndim, tl->numtiles, NULL, 0, cp->minmapsize, NULL, p->input->unit, NULL); qprm.noerode_th=gal_data_alloc(NULL, p->input->type, p->input->ndim, tl->numtiles, NULL, 0, cp->minmapsize, NULL, p->input->unit, NULL); if(p->detgrowquant!=1.0f) qprm.expand_th=gal_data_alloc(NULL, p->input->type, p->input->ndim, tl->numtiles, NULL, 0, cp->minmapsize, NULL, p->input->unit, NULL); else qprm.expand_th=NULL; /* Allocate temporary space for processing in each tile. */ qprm.usage=gal_data_malloc_array(p->input->type, cp->numthreads * p->maxtcontig, __func__, "qprm.usage"); /* Find the threshold on each tile, free the temporary processing space and set the blank flag on both. Since they have the same blank elements, it is only necessary to check one (with the `updateflag' value set to 1), then update the next. */ qprm.p=p; gal_threads_spin_off(qthresh_on_tile, &qprm, tl->tottiles, cp->numthreads); free(qprm.usage); if( gal_blank_present(qprm.erode_th, 1) ) { qprm.noerode_th->flag |= GAL_DATA_FLAG_HASBLANK; if(qprm.expand_th) qprm.expand_th->flag |= GAL_DATA_FLAG_HASBLANK; } qprm.noerode_th->flag |= GAL_DATA_FLAG_BLANK_CH; if(p->detgrowquant!=1.0f) qprm.expand_th->flag |= GAL_DATA_FLAG_BLANK_CH; if(p->qthreshname) { qprm.erode_th->name="QTHRESH_ERODE"; qprm.noerode_th->name="QTHRESH_NOERODE"; gal_tile_full_values_write(qprm.erode_th, tl, 1, p->qthreshname, NULL, PROGRAM_NAME); gal_tile_full_values_write(qprm.noerode_th, tl, 1, p->qthreshname, NULL, PROGRAM_NAME); qprm.erode_th->name=qprm.noerode_th->name=NULL; if(qprm.expand_th) { qprm.expand_th->name="QTHRESH_EXPAND"; gal_tile_full_values_write(qprm.expand_th, tl, 1, p->qthreshname, NULL, PROGRAM_NAME); qprm.expand_th->name=NULL; } } /* Remove higher thresholds if requested. */ if(p->qthreshtilequant!=1.0) threshold_qthresh_clean(p, qprm.erode_th, qprm.noerode_th, qprm.expand_th ? qprm.expand_th : NULL, p->qthreshname); /* Interpolate and smooth the derived values. */ threshold_interp_smooth(p, &qprm.erode_th, &qprm.noerode_th, qprm.expand_th ? &qprm.expand_th : NULL, p->qthreshname); /* We now have a threshold for all tiles, apply it. */ threshold_apply(p, qprm.erode_th->array, qprm.noerode_th->array, THRESHOLD_QUANTILES); /* Write the binary image if check is requested. */ if(p->qthreshname && !tl->oneelempertile) gal_fits_img_write(p->binary, p->qthreshname, NULL, PROGRAM_NAME); /* Set the expansion quantile if necessary. */ p->expand_thresh = qprm.expand_th ? qprm.expand_th : NULL; /* Clean up and report duration if necessary. */ gal_data_free(qprm.erode_th); gal_data_free(qprm.noerode_th); if(!p->cp.quiet) { asprintf(&msg, "%.2f & %0.2f quantile thresholds applied.", p->qthresh, p->noerodequant); gal_timing_report(&t1, msg, 2); free(msg); } /* If the user wanted to check the threshold and hasn't called `continueaftercheck', then stop NoiseChisel. */ if(p->qthreshname && !p->continueaftercheck) ui_abort_after_check(p, p->qthreshname, NULL, "quantile threshold check"); } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/segmentation.c���������������������������������������������������������0000644�0001750�0001750�00000076337�13205003172�016070� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/binary.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "ui.h" #include "clumps.h" #include "segmentation.h" /***********************************************************************/ /***************** Relabeling (grown) clumps *****************/ /***********************************************************************/ /* Correct the label of an detection when it doesn't need segmentation (it is fully one object). The final labels for the object(s) with a detected region will be set later (don't forget that we have detections that are composed of multiple objects). So the labels within each detection start from 1.*/ static void segmentation_relab_noseg(struct clumps_thread_params *cltprm) { int32_t *olabel=cltprm->clprm->p->olabel->array; size_t *s=cltprm->indexs->array, *sf=s+cltprm->indexs->size; do olabel[ *s ] = 1; while(++s<sf); } /* Find the adjacency matrixs (number, sum and signal to noise) for the rivers between potentially separate objects in a detection region. They have to be allocated prior to entering this funciton. The way to find connected objects is through an adjacency matrix. It is a square matrix with a side equal to numobjs. So to see if regions `a` and `b` are connected. All we have to do is to look at element a*numobjs+b or b*numobjs+a and get the answer. Since the number of objects in a given region will not be too high, this is efficient. */ static void segmentation_relab_to_objects(struct clumps_thread_params *cltprm) { size_t amwidth=cltprm->numtrueclumps+1; struct noisechiselparams *p=cltprm->clprm->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; size_t mdsize[2]={amwidth, amwidth}; gal_data_t *nums_d=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 2, mdsize, NULL, 1, p->cp.minmapsize, NULL, NULL, NULL); gal_data_t *sums_d=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 2, mdsize, NULL, 1, p->cp.minmapsize, NULL, NULL, NULL); gal_data_t *adjacency_d=gal_data_alloc(NULL, GAL_TYPE_UINT8, 2, mdsize, NULL, 1, p->cp.minmapsize, NULL, NULL, NULL); float *imgss=p->input->array; uint8_t *adjacency=adjacency_d->array; size_t nngb=gal_dimension_num_neighbors(ndim); int32_t *clumptoobj, *olabel=p->olabel->array; size_t *dinc=gal_dimension_increment(ndim, dsize); size_t *s, *sf, i, j, ii, rpnum, *nums=nums_d->array; double ave, rpsum, c=sqrt(1/p->cpscorr), *sums=sums_d->array; double err=cltprm->std*cltprm->std*(p->skysubtracted?1.0f:2.0f); int32_t *ngblabs=gal_data_malloc_array(GAL_TYPE_UINT32, nngb, __func__, "ngblabs"); /* Go over all the still-unlabeled pixels (if they exist) and see which labels they touch. In the process, get the average value of the river-pixel values and put them in the respective adjacency matrix. Note that at this point, the rivers are also part of the "diffuse" regions. So we don't need to go over all the indexs of this object, only its diffuse indexs. */ if(cltprm->diffuseindexs->size) { sf=(s=cltprm->diffuseindexs->array)+cltprm->diffuseindexs->size; do /* We only want to work on pixels that have already been identified as touching more than one label: river pixels. */ if( olabel[ *s ]==CLUMPS_RIVER ) { /* Initialize the values. */ i=ii=0; rpnum=1; /* River-pixel number of points used. */ rpsum=imgss[*s]; /* River-pixel sum of values used. */ memset(ngblabs, 0, nngb*sizeof *ngblabs); /* Check all the fully-connected neighbors of this pixel and see if it touches a label or not */ GAL_DIMENSION_NEIGHBOR_OP(*s, ndim, dsize, ndim, dinc, { if( olabel[nind] > 0 ) { /* Add this neighbor's value and increment the number. */ if( !isnan(imgss[nind]) ) { ++rpnum; rpsum+=imgss[nind]; } /* Go over the already found neighbors and see if this grown clump has already been considered or not. */ for(i=0;i<ii;++i) if(ngblabs[i]==olabel[nind]) break; /* This is the first time we are getting to this neighbor: */ if(i==ii) ngblabs[ ii++ ] = olabel[nind]; } } ); /* For a check: if(ii>0) { printf("%zu, %zu:\n", *s%dsize[1]+1, *s/dsize[1]+1); for(i=0;i<ii;++i) printf("\t%u\n", ngblabs[i]); } */ /* If more than one neighboring label was found, fill in the 'sums' and 'nums' adjacency matrixs with the values for this pixel. Recall that ii is the number of neighboring labels to this river pixel. */ if(ii>i) for(i=0;i<ii;++i) for(j=0;j<ii;++j) if(i!=j) { /* For safety, we will fill both sides of the diagonal. */ ++nums[ ngblabs[i] * amwidth + ngblabs[j] ]; ++nums[ ngblabs[j] * amwidth + ngblabs[i] ]; sums[ ngblabs[i] * amwidth + ngblabs[j] ] += rpsum/rpnum; sums[ ngblabs[j] * amwidth + ngblabs[i] ] += rpsum/rpnum; } } while(++s<sf); /* We now have the average values and number of all rivers between the grown clumps. We now want to finalize their connection (given the user's criteria). */ for(i=1;i<amwidth;++i) for(j=1;j<i;++j) { ii = i * amwidth + j; if(nums[ii]>p->minriverlength) /* There is a connection. */ { /* For easy reading. */ ave=sums[ii]/nums[ii]; /* In case the average is negative (only possible if `sums' is negative), don't change the adjacency: it is already initialized to zero. Note that even an area of 1 is acceptable, and we put no area criteria here, because the fact that a river exists between two clumps is important. */ if( ave>0.0f && ( c * ave / sqrt(ave+err) ) > p->objbordersn ) { adjacency[ii]=1; /* We want to set both sides of the */ adjacency[ j * amwidth + i ] = 1; /* Symmetric matrix. */ } } } /* For a check: if(cltprm->id==XXX) { printf("=====================\n"); printf("%zu:\n--------\n", cltprm->id); for(i=1;i<amwidth;++i) { printf(" %zu...\n", i); for(j=1;j<amwidth;++j) { ii=i*amwidth+j; if(nums[ii]) { ave=sums[ii]/nums[ii]; printf(" ...%zu: N:%-4zu S:%-10.2f S/N: %-10.2f " "--> %u\n", j, nums[ii], sums[ii], c*ave/sqrt(ave+err), adjacency[ii]); } } printf("\n"); } } */ /* Calculate the new labels for each grown clump. */ cltprm->clumptoobj = gal_binary_connected_adjacency_matrix(adjacency_d, &cltprm->numobjects); clumptoobj = cltprm->clumptoobj->array; } /* There was no list of diffuse pixels, this happens when the user sets a very high `gthresh' threshold and wants to make sure that each clump is a separate object. So we need to define the number of objects and `clumptoobj' manually. */ else { /* Allocate the `clumptoobj' array. */ cltprm->clumptoobj = gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &amwidth, NULL, 1, p->cp.minmapsize, NULL, NULL, NULL); clumptoobj = cltprm->clumptoobj->array; /* Fill in the `clumptoobj' array with the indexs of the objects. */ for(i=0;i<amwidth;++i) clumptoobj[i]=i; /* Set the number of objects. */ cltprm->numobjects = cltprm->numtrueclumps; } /* For a check if(cltprm->id==XXXX) { printf("NUMTRUECLUMPS: %zu\n----------\n", cltprm->numtrueclumps); for(i=0;i<cltprm->numtrueclumps+1;++i) printf("\t%zu --> %d\n", i, clumptoobj[i]); printf("=== numobjects: %zu====\n", cltprm->numobjects); exit(0); } */ /* Correct all the labels. */ sf=(s=cltprm->indexs->array)+cltprm->indexs->size; do if( olabel[*s] > 0 ) olabel[*s] = clumptoobj[ olabel[*s] ]; while(++s<sf); /* Clean up and return. */ free(dinc); free(ngblabs); gal_data_free(nums_d); gal_data_free(sums_d); gal_data_free(adjacency_d); } /* The correspondance between the clumps and objects has been found. With this function, we want to correct the clump labels so the clump IDs in each object start from 1 and are contiguous. */ static void segmentation_relab_clumps_in_objects(struct clumps_thread_params *cltprm) { size_t numobjects=cltprm->numobjects, numtrueclumps=cltprm->numtrueclumps; int32_t *clumptoobj=cltprm->clumptoobj->array; int32_t *clabel=cltprm->clprm->p->clabel->array; size_t i, *s=cltprm->indexs->array, *sf=s+cltprm->indexs->size; size_t *nclumpsinobj=gal_data_calloc_array(GAL_TYPE_SIZE_T, numobjects+1, __func__, "nclumpsinobj"); int32_t *newlabs=gal_data_calloc_array(GAL_TYPE_UINT32, numtrueclumps+1, __func__, "newlabs"); /* Fill both arrays. */ for(i=1;i<numtrueclumps+1;++i) newlabs[i] = ++nclumpsinobj[ clumptoobj[i] ]; /* Reset the clump labels over the detection region. */ do if(clabel[*s]>0) clabel[*s] = newlabs[ clabel[*s] ]; while(++s<sf); /* Clean up. */ free(newlabs); free(nclumpsinobj); } /* Prior to this function, the objects have labels that are unique and contiguous (the labels are contiguous, not the objects!) within each detection and start from 1. However, for the final output, it is necessary that each object over the whole dataset have a unique ID. Since multiple threads are working on separate objects at every instance, this function will use a mutex to limit the reading and writing to the variable keeping the total number of objects counter. */ static void segmentation_relab_overall(struct clumps_thread_params *cltprm) { struct clumps_params *clprm=cltprm->clprm; int32_t startinglab, *olabel=clprm->p->olabel->array; size_t *s=cltprm->indexs->array, *sf=s+cltprm->indexs->size; /* Lock the mutex if we are working on more than one thread. NOTE: it is very important to keep the number of operations within the mutex to a minimum so other threads don't get delayed. */ if(clprm->p->cp.numthreads>1) pthread_mutex_lock(&clprm->labmutex); /* Save the total number of objects found so far into `startinglab', then increment the total number of objects and clumps. */ startinglab = clprm->totobjects; clprm->totobjects += cltprm->numobjects; clprm->totclumps += cltprm->numtrueclumps; /* Unlock the mutex (if it was locked). */ if(clprm->p->cp.numthreads>1) pthread_mutex_unlock(&clprm->labmutex); /* Increase all the object labels by `startinglab'. */ do olabel[*s] += startinglab; while(++s<sf); } /***********************************************************************/ /***************** Over detections *****************/ /***********************************************************************/ /* Find the true clumps over each detection. */ static void * segmentation_on_threads(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct clumps_params *clprm=(struct clumps_params *)(tprm->params); struct noisechiselparams *p=clprm->p; size_t i, *s, *sf; gal_data_t *topinds; struct clumps_thread_params cltprm; int32_t *clabel=p->clabel->array, *olabel=p->olabel->array; /* Initialize the general parameters for this thread. */ cltprm.clprm = clprm; /* Go over all the detections given to this thread (counting from zero.) */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* Set the ID of this detection, note that for the threads, we counted from zero, but the IDs start from 1, so we'll add a 1 to the ID given to this thread. */ cltprm.id = tprm->indexs[i]+1; cltprm.indexs = &clprm->labindexs[ cltprm.id ]; /* The `topinds' array is only necessary when the user wants to ignore true clumps with a peak touching a river. */ if(p->keepmaxnearriver==0) { /* Allocate the list of local maxima. For each clump there is going to be one local maxima. But we don't know the number of clumps a-priori, so we'll just allocate the number of pixels given to this detected region. */ topinds=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 1, cltprm.indexs->dsize, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); cltprm.topinds=topinds->array; } else { cltprm.topinds=NULL; topinds=NULL; } /* Find the clumps over this region. */ clumps_oversegment(&cltprm); /* Make the clump S/N table. This table is made before (possibly) stopping the process (if a check is requested). This is because if the user has also asked for a check image, we can break out of the loop at that point. Note that the array of `gal_data_t' that keeps the S/N table for each detection is allocated before threading starts. However, when the user wants to inspect the steps, this function is called multiple times. So we need to avoid over-writing the allocations. */ if( clprm->sn[ cltprm.id ].dsize==NULL ) clumps_make_sn_table(&cltprm); else cltprm.sn=&clprm->sn[ cltprm.id ]; /* If the user wanted to check the segmentation steps or the clump S/N values in a table, then we have to stop the process at this point. */ if(clprm->step==1 || p->checkclumpsn) { gal_data_free(topinds); continue; } /* Only keep true clumps. */ clumps_det_keep_true_relabel(&cltprm); gal_data_free(topinds); if(clprm->step==2) continue; /* Set the internal (with the detection) clump and object labels. Segmenting a detection into multiple objects is only defined when there is more than one true clump over the detection. When there is only one true clump (cltprm->numtrueclumps==1) or none (p->numtrueclumps==0), then just set the required preliminaries to make the next steps be generic for all cases. */ if(cltprm.numtrueclumps<=1) { /* Set the basics. */ cltprm.numobjects=1; segmentation_relab_noseg(&cltprm); /* If the user wanted a check image, this object doesn't change. */ if( clprm->step >= 3 && clprm->step <= 6) continue; /* If the user has asked for grown clumps in the clumps image instead of the raw clumps, then replace the indexs in the `clabel' array is well. In this case, there will always be one "clump". */ if(p->grownclumps) { sf=(s=cltprm.indexs->array)+cltprm.indexs->size; do clabel[ *s++ ] = 1; while(s<sf); cltprm.numtrueclumps=1; } } else { /* Grow the true clumps over the detection. */ clumps_grow_prepare_initial(&cltprm); if(cltprm.diffuseindexs->size) clumps_grow(p->olabel, cltprm.diffuseindexs, 1, 1); if(clprm->step==3) { gal_data_free(cltprm.diffuseindexs); continue; } /* If grown clumps are desired instead of the raw clumps, then replace all the grown clumps with those in clabel. */ if(p->grownclumps) { sf=(s=cltprm.indexs->array)+cltprm.indexs->size; do if(olabel[*s]>0) clabel[*s]=olabel[*s]; while(++s<sf); } /* Identify the objects in this detection using the grown clumps and correct the grown clump labels into new object labels. */ segmentation_relab_to_objects(&cltprm); if(clprm->step==4) { gal_data_free(cltprm.clumptoobj); gal_data_free(cltprm.diffuseindexs); continue; } /* Continue the growth and cover the whole area, we don't need the diffuse indexs any more, so after filling the detected region, free the indexs. */ if( cltprm.numobjects == 1 ) segmentation_relab_noseg(&cltprm); else { /* Correct the labels so every non-labeled pixel can be grown. */ clumps_grow_prepare_final(&cltprm); /* Cover the whole area (using maximum connectivity to not miss any pixels). */ clumps_grow(p->olabel, cltprm.diffuseindexs, 0, p->olabel->ndim); /* Make sure all diffuse pixels are labeled. */ if(cltprm.diffuseindexs->size) error(EXIT_FAILURE, 0, "a bug! Please contact us at %s to " "fix it. %zu pixels of detection %zu have not been " "labeled (as an object)", PACKAGE_BUGREPORT, cltprm.diffuseindexs->size, cltprm.id); } gal_data_free(cltprm.diffuseindexs); if(clprm->step==5) { gal_data_free(cltprm.clumptoobj); continue; } /* Correct the clump labels. Note that this is only necessary when there is more than object over the detection or when there were multiple clumps over the detection. */ if(cltprm.numobjects>1) segmentation_relab_clumps_in_objects(&cltprm); gal_data_free(cltprm.clumptoobj); if(clprm->step==6) {continue;} } /* Convert the object labels to their final value */ segmentation_relab_overall(&cltprm); } /* Wait until all the threads finish then return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* If the user wanted to see the S/N table in a file, this function will be called and will do the job. */ static void segmentation_save_sn_table(struct clumps_params *clprm) { char *msg; float *sarr; int32_t *oiarr, *cioarr; gal_list_str_t *comments=NULL; size_t i, j, c=0, totclumps=0; gal_data_t *sn, *objind, *clumpinobj; struct noisechiselparams *p=clprm->p; /* Find the total number of clumps in all the initial detections. Recall that the `size' values were one more than the actual number because the labelings start from 1. */ for(i=1;i<p->numdetections+1;++i) totclumps += clprm->sn[i].size-1; /* Allocate the columns for the table. */ sn=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &totclumps, NULL, 0, p->cp.minmapsize, "CLUMP_S/N", "ratio", "Signal-to-noise ratio."); objind=gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &totclumps, NULL, 0, p->cp.minmapsize, "HOST_DET_ID", "counter", "ID of detection hosting this clump."); clumpinobj=gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &totclumps, NULL, 0, p->cp.minmapsize, "CLUMP_ID_IN_OBJ", "counter", "ID of clump in host detection."); /* Fill in the columns. */ sarr=sn->array; oiarr=objind->array; cioarr=clumpinobj->array; for(i=1;i<p->numdetections+1;++i) for(j=1;j<clprm->sn[i].size;++j) { oiarr[c] = i; cioarr[c] = j; sarr[c] = ((float *)(clprm->sn[i].array))[j]; ++c; } /* Write the comments. */ gal_list_str_add(&comments, "See also: `CLUMPS_ALL_DET' HDU of " "output with `--checksegmentation'.", 1); asprintf(&msg, "S/N values of `nan': clumps smaller than `--segsnminarea' " "of %zu.", p->segsnminarea); gal_list_str_add(&comments, msg, 0); gal_list_str_add(&comments, "S/N of clumps over detected regions.", 1); gal_table_comments_add_intro(&comments, PROGRAM_STRING, &p->rawtime); /* Set the column pointers and write them into a table.. */ clumpinobj->next=sn; objind->next=clumpinobj; gal_checkset_writable_remove(p->clumpsn_d_name, 0, 1); gal_table_write(objind, comments, p->cp.tableformat, p->clumpsn_d_name, "CLUMPS_SN"); /* Clean up. */ gal_data_free(sn); gal_data_free(objind); gal_data_free(clumpinobj); gal_list_str_free(comments, 1); /* Abort NoiseChisel if necessary. */ if(!p->continueaftercheck) ui_abort_after_check(p, p->clumpsn_s_name, p->clumpsn_d_name, "showing all clump S/N values"); } /* Find true clumps over the detected regions. */ static void segmentation_detections(struct noisechiselparams *p) { char *msg; struct clumps_params clprm; gal_data_t *labindexs, *claborig, *demo=NULL; /* Get the indexs of all the pixels in each label. */ labindexs=clumps_det_label_indexs(p); /* Initialize the necessary thread parameters. Note that since the object labels begin from one, the `sn' array will have one extra element.*/ clprm.p=p; clprm.sky0_det1=1; clprm.totclumps=0; clprm.totobjects=0; clprm.snind = NULL; clprm.labindexs=labindexs; clprm.sn=gal_data_array_calloc(p->numdetections+1); /* When more than one thread is to be used, initialize the mutex. */ if( p->cp.numthreads > 1 ) pthread_mutex_init(&clprm.labmutex, NULL); /* Spin off the threads to start the work. Note that several steps are done on each tile within a thread. So if the user wants to check steps, we need to break out of the processing get an over-all output, then reset the input and call it again. So it will be slower, but its is natural, since the user is testing to find the correct combination of parameters for later use. */ if(p->segmentationname) { /* Necessary initializations. */ clprm.step=1; claborig=p->clabel; p->clabel=gal_data_copy(claborig); /* Do each step. */ while(clprm.step<8) { /* Reset the temporary copy of clabel back to its original. */ if(clprm.step>1) memcpy(p->clabel->array, claborig->array, claborig->size*gal_type_sizeof(claborig->type)); /* (Re-)do everything until this step. */ gal_threads_spin_off(segmentation_on_threads, &clprm, p->numdetections, p->cp.numthreads); /* Set the extension name. */ switch(clprm.step) { case 1: demo=p->clabel; demo->name = "DET_CLUMPS_ALL"; if(!p->cp.quiet) { asprintf(&msg, "Identified clumps over detections " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; case 2: demo=p->clabel; demo->name = "DET_CLUMPS_TRUE"; if(!p->cp.quiet) { asprintf(&msg, "True clumps found " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; case 3: demo=p->olabel; demo->name = "DET_CLUMPS_GROWN"; if(!p->cp.quiet) { gal_timing_report(NULL, "Starting to identify objects.", 1); asprintf(&msg, "True clumps grown " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; case 4: demo=p->olabel; demo->name = "DET_OBJ_IDENTIFIED"; if(!p->cp.quiet) { asprintf(&msg, "Identified objects over detections " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; case 5: demo=p->olabel; demo->name = "DET_OBJECTS_FULL"; if(!p->cp.quiet) { asprintf(&msg, "Objects grown to cover full area " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; case 6: demo=p->clabel; demo->name = "CLUMPS_FINAL"; if(!p->cp.quiet) { asprintf(&msg, "Clumps given their final label " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; case 7: demo=p->olabel; demo->name = "OBJECTS_FINAL"; if(!p->cp.quiet) { asprintf(&msg, "Objects given their final label " "(HDU: `%s').", demo->name); gal_timing_report(NULL, msg, 2); free(msg); } break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so " "we can address the issue. The value %d is not " "recognized for clprm.step", __func__, PACKAGE_BUGREPORT, clprm.step); } /* Write the demonstration array into the check image. The default values are hard to view, so we'll make a copy of the demo, set all Sky regions to blank and all clump macro values to zero. */ gal_fits_img_write(demo, p->segmentationname, NULL, PROGRAM_NAME); /* If the user wanted to check the clump S/N values, then break out of the loop, we don't need the rest of the process any more. */ if( clprm.step==1 && ( p->checkclumpsn && !p->continueaftercheck ) ) break; /* Increment the step counter. */ ++clprm.step; } /* Clean up (we don't need the original any more). */ gal_data_free(claborig); p->olabel->name = p->clabel->name = NULL; } else { clprm.step=0; gal_threads_spin_off(segmentation_on_threads, &clprm, p->numdetections, p->cp.numthreads); } /* Save the final number of objects and clumps. */ p->numclumps=clprm.totclumps; p->numobjects=clprm.totobjects; /* If the user wanted to see the S/N table, then make the S/N table. */ if(p->checkclumpsn) segmentation_save_sn_table(&clprm); /* Clean up allocated structures and destroy the mutex. */ gal_data_array_free(clprm.sn, p->numdetections+1, 1); gal_data_array_free(labindexs, p->numdetections+1, 1); if( p->cp.numthreads>1 ) pthread_mutex_destroy(&clprm.labmutex); } /***********************************************************************/ /***************** High level function *****************/ /***********************************************************************/ void segmentation(struct noisechiselparams *p) { float *f; char *msg; int32_t *l, *lf; struct timeval t1; /* To keep the user up to date. */ if(!p->cp.quiet) { if(!p->cp.quiet) gettimeofday(&t1, NULL); gal_timing_report(NULL, "Starting segmentation.", 1); } /* If a check segmentation image was requested, then put in the inputs. */ if(p->segmentationname) { gal_fits_img_write(p->input, p->segmentationname, NULL, PROGRAM_NAME); gal_fits_img_write(p->conv, p->segmentationname, NULL, PROGRAM_NAME); p->olabel->name="DETECTION_LABELS"; gal_fits_img_write(p->olabel, p->segmentationname, NULL, PROGRAM_NAME); p->olabel->name=NULL; } /* Allocate the clump labels image. */ p->clabel=gal_data_alloc(NULL, p->olabel->type, p->olabel->ndim, p->olabel->dsize, p->olabel->wcs, 1, p->cp.minmapsize, NULL, NULL, NULL); p->clabel->flag=p->input->flag; /* Set any possibly existing NaN values to blank. */ f=p->input->array; lf=(l=p->clabel->array)+p->clabel->size; do if(isnan(*f++)) *l=GAL_BLANK_INT32; while(++l<lf); /* Find the clump S/N threshold. */ clumps_true_find_sn_thresh(p); /* Reset the clabel array to find true clumps in objects. */ f=p->input->array; lf=(l=p->clabel->array)+p->clabel->size; do *l = isnan(*f++) ? GAL_BLANK_INT32 : 0; while(++l<lf); /* Find true clumps over the detected regions. */ segmentation_detections(p); /* Report the results and timing to the user. */ if(!p->cp.quiet) { asprintf(&msg, "%zu object%s""containing %zu clump%sfound.", p->numobjects, p->numobjects==1 ? " " : "s ", p->numclumps, p->numclumps ==1 ? " " : "s "); gal_timing_report(&t1, msg, 1); free(msg); } /* If the user wanted to check the segmentation and hasn't called `continueaftercheck', then stop NoiseChisel. */ if(p->segmentationname && !p->continueaftercheck) ui_abort_after_check(p, p->segmentationname, NULL, "showing all segmentation steps"); } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/sky.c������������������������������������������������������������������0000644�0001750�0001750�00000021253�13156610402�014171� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <gnuastro/tile.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/threads.h> #include <gnuastro/statistics.h> #include "main.h" #include "ui.h" #include "threshold.h" /**************************************************************** ************ Estimate the Sky ************ ****************************************************************/ static void * sky_mean_std_undetected(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct noisechiselparams *p=(struct noisechiselparams *)tprm->params; double *darr, s, s2; int type=p->sky->type; size_t i, tind, numsky, dsize=2; gal_data_t *tile, *meanstd_d, *meanstd, *bintile; /* A dataset to keep the mean and STD in double type. */ meanstd_d=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); darr=meanstd_d->array; /* An empty dataset to replicate a tile on the binary array. */ bintile=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &dsize, NULL, 0, -1, NULL, NULL, NULL); free(bintile->array); free(bintile->dsize); bintile->block=p->binary; bintile->ndim=p->binary->ndim; /* Go over all the tiles given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* Basic definitions */ numsky=0; tind = tprm->indexs[i]; tile = &p->cp.tl.tiles[tind]; /* Correct the fake binary tile's properties to be the same as this one, then count the number of zero valued elements in it. */ bintile->size=tile->size; bintile->dsize=tile->dsize; bintile->array=gal_tile_block_relative_to_other(tile, p->binary); GAL_TILE_PARSE_OPERATE(tile, bintile, 1, 1, {if(!*o) numsky++;}); /* Only continue, if the fraction of Sky values are less than the requested fraction. */ if( (float)(numsky)/(float)(tile->size) > p->minskyfrac) { /* Calculate the mean and STD over this tile. */ s=s2=0.0f; GAL_TILE_PARSE_OPERATE(tile, bintile, 1, 1, { if(!*o) { s += *i; s2 += *i * *i; } } ); darr[0]=s/numsky; darr[1]=sqrt( (s2-s*s/numsky)/numsky ); /* Convert the mean and std into the same type as the sky and std arrays. */ meanstd=gal_data_copy_to_new_type(meanstd_d, type); /* Copy the mean and STD to their respective places in the tile arrays. */ memcpy(gal_data_ptr_increment(p->sky->array, tind, type), meanstd->array, gal_type_sizeof(type)); memcpy(gal_data_ptr_increment(p->std->array, tind, type), gal_data_ptr_increment(meanstd->array, 1, type), gal_type_sizeof(type)); /* Clean up. */ gal_data_free(meanstd); } else { gal_blank_write(gal_data_ptr_increment(p->sky->array, tind, type), type); gal_blank_write(gal_data_ptr_increment(p->std->array, tind, type), type); } } /* Clean up and wait for other threads to finish and abort. */ bintile->array=NULL; bintile->dsize=NULL; gal_data_free(bintile); gal_data_free(meanstd_d); if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } void sky_and_std(struct noisechiselparams *p, char *checkname) { gal_data_t *tmp; struct gal_options_common_params *cp=&p->cp; struct gal_tile_two_layer_params *tl=&cp->tl; /* When the check image has the same resolution as the input, write the binary array as a reference to help in the comparison. */ if(checkname && !tl->oneelempertile) { p->binary->name="DETECTED"; gal_fits_img_write(p->binary, checkname, NULL, PROGRAM_NAME); p->binary->name=NULL; } /* Allocate space for the mean and standard deviation. */ p->sky=gal_data_alloc(NULL, p->input->type, p->input->ndim, tl->numtiles, NULL, 0, cp->minmapsize, "SKY", p->input->unit, NULL); p->std=gal_data_alloc(NULL, p->input->type, p->input->ndim, tl->numtiles, NULL, 0, cp->minmapsize, "STD", p->input->unit, NULL); /* Find the Sky and its STD on proper tiles. */ gal_threads_spin_off(sky_mean_std_undetected, p, tl->tottiles, cp->numthreads); if(checkname) { gal_tile_full_values_write(p->sky, tl, 1, checkname, NULL, PROGRAM_NAME); gal_tile_full_values_write(p->std, tl, 1, checkname, NULL, PROGRAM_NAME); } /* Get the basic information about the standard deviation distribution. */ tmp=gal_statistics_median(p->std, 0); tmp=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); memcpy(&p->medstd, tmp->array, sizeof p->medstd); gal_data_free(tmp); tmp=gal_statistics_minimum(p->std); tmp=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); memcpy(&p->minstd, tmp->array, sizeof p->minstd); gal_data_free(tmp); tmp=gal_statistics_maximum(p->std); tmp=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); memcpy(&p->maxstd, tmp->array, sizeof p->maxstd); gal_data_free(tmp); /* In case the image is in electrons or counts per second, the standard deviation of the noise will become smaller than unity, so we need to correct it in the S/N calculation. So, we'll calculate the correction factor here. */ p->cpscorr = p->minstd>1 ? 1.0f : p->minstd; /* Interpolate and smooth the derived values. */ threshold_interp_smooth(p, &p->sky, &p->std, NULL, checkname); /* If a check was requested, abort NoiseChisel. */ if(checkname && !p->continueaftercheck) ui_abort_after_check(p, checkname, NULL, "showing derivation of Sky " "value and its standard deviation, or STD"); } /**************************************************************** ************ Subtract the Sky ************ ****************************************************************/ void sky_subtract(struct noisechiselparams *p) { size_t tid; void *tarray=NULL; float *sky=p->sky->array; gal_data_t *tile, *tblock=NULL; /* A small sanity check. */ if(p->sky->type!=GAL_TYPE_FLOAT32) error(EXIT_FAILURE, 0, "%s: only `float32' type is acceptable " "for sky values. but `p->sky' has type `%s'", __func__, gal_type_name(p->sky->type, 1)); /* Go over all the tiles. */ for(tid=0; tid<p->cp.tl.tottiles; ++tid) { /* For easy reading. */ tile=&p->cp.tl.tiles[tid]; /* First subtract the Sky value from the input image. */ GAL_TILE_PARSE_OPERATE(tile, NULL, 0, 0, {*i-=sky[tid];}); /* Change to the convolved image. */ tarray=tile->array; tblock=tile->block; tile->array=gal_tile_block_relative_to_other(tile, p->conv); tile->block=p->conv; /* The threshold is always low. So for the majority of non-NaN pixels in the image, the condition above will be true. If we come over a NaN pixel, then by definition of NaN, all conditionals will fail. If an image doesn't have any NaN pixels, only the pixels below the threshold have to be checked for a NaN which are by definition a very small fraction of the total pixels. And if there are NaN pixels in the image. */ GAL_TILE_PARSE_OPERATE(tile, NULL, 0, 0, {*i-=sky[tid];}); /* Revert back to the original block. */ tile->array=tarray; tile->block=tblock; } } �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/noisechisel.c����������������������������������������������������������0000644�0001750�0001750�00000022777�13177434336�015721� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/convolve.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "ui.h" #include "sky.h" #include "detection.h" #include "threshold.h" #include "segmentation.h" /***********************************************************************/ /************* Wrapper functions (for clean high-level) ***************/ /***********************************************************************/ static void noisechisel_convolve(struct noisechiselparams *p) { struct timeval t1; struct gal_tile_two_layer_params *tl=&p->cp.tl; /* Convovle with sharper kernel. */ if(p->conv==NULL) { /* Make the convolved image. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); p->conv = gal_convolve_spatial(tl->tiles, p->kernel, p->cp.numthreads, 1, tl->workoverch); /* Report and write check images if necessary. */ if(!p->cp.quiet) { if(p->widekernel) gal_timing_report(&t1, "Convolved with sharper kernel.", 1); else gal_timing_report(&t1, "Convolved with given kernel.", 1); } } /* Set a fixed name for the convolved image (since it will be used in many check images). */ if(p->conv->name) free(p->conv->name); gal_checkset_allocate_copy( ( p->widekernel ? "CONVOLVED-SHARPER" : "CONVOLVED" ), &p->conv->name); /* Save the convolution step if necessary. */ if(p->detectionname) { gal_fits_img_write(p->input, p->detectionname, NULL, PROGRAM_NAME); gal_fits_img_write(p->conv, p->detectionname, NULL, PROGRAM_NAME); } /* Convolve with wider kernel (if requested). */ if(p->widekernel) { if(!p->cp.quiet) gettimeofday(&t1, NULL); p->wconv=gal_convolve_spatial(tl->tiles, p->widekernel, p->cp.numthreads, 1, tl->workoverch); gal_checkset_allocate_copy("CONVOLVED-WIDER", &p->wconv->name); if(!p->cp.quiet) gal_timing_report(&t1, "Convolved with wider kernel.", 1); } } static void noisechisel_find_sky_subtract(struct noisechiselparams *p) { /* Find the final Sky value. */ sky_and_std(p, p->skyname); /* Abort if the user only wanted to see until this point.*/ if(p->skyname && !p->continueaftercheck) ui_abort_after_check(p, p->skyname, NULL, "derivation of final Sky (and its STD) value"); /* Subtract the Sky from the Input and Convolved (necessary for segmentation) images. */ sky_subtract(p); } /* If convolution was not done while respecting channel edges (when there is more than one channel, pixels outside the edge weren't used in the convolution), then correct it. */ static void noisechisel_convolve_correct_ch_edges(struct noisechiselparams *p) { struct gal_tile_two_layer_params *tl=&p->cp.tl; /* Correct the convolved image if necessary. */ if( tl->totchannels>1 && tl->workoverch==0 ) { /* Do the correction. */ gal_convolve_spatial_correct_ch_edge(tl->tiles, p->kernel, p->cp.numthreads, 1, p->conv); /* Inform the user. */ if(!p->cp.quiet) gal_timing_report(NULL, "Corrected convolution of touching channel " "edges", 1); } } /***********************************************************************/ /************* Output ***************/ /***********************************************************************/ /* The input image has been sky subtracted for further processing. So we'll need to copy the input image directly into the output. */ static void noisechisel_output_copy_input(struct noisechiselparams *p) { int status=0; fitsfile *in, *out; char card[FLEN_CARD]; /* Create/open the output file. */ out=gal_fits_open_to_write(p->cp.output); /* Open the input FITS file in the proper extension. */ in=gal_fits_hdu_open(p->inputname, p->cp.hdu, READWRITE); /* Copy the input HDU into the output. */ if( fits_copy_hdu(in, out, 0, &status) ) gal_fits_io_error(status, "copying input hdu into first output hdu"); /* If an extension name exists in the input HDU, then don't touch it. If the input doesn't have any, then make an EXTNAME keyword for it. Note that `fits_read_card' will return a non-zero if it doesn't find the keyword. */ if( fits_read_card(out, "EXTNAME", card, &status) ) { status=0; fits_write_key(out, TSTRING, "EXTNAME", "INPUT", "", &status); } /* Close the two files. */ fits_close_file(in, &status); fits_close_file(out, &status); } /* Write the output file. */ static void noisechisel_output(struct noisechiselparams *p) { gal_fits_list_key_t *keys=NULL; /* Copy the input image into the first extension. */ noisechisel_output_copy_input(p); /* Write the object labels and useful information into it's header. */ if(p->onlydetection==0) gal_fits_key_list_add(&keys, GAL_TYPE_STRING, "WCLUMPS", 0, "yes", 0, "Generate catalog with clumps?", 0, "bool"); gal_fits_key_list_add(&keys, GAL_TYPE_SIZE_T, "NUMLABS", 0, &p->numobjects, 0, "Total number of labels " "(inclusive)", 0, "counter"); gal_fits_key_list_add(&keys, GAL_TYPE_FLOAT32, "DETSN", 0, &p->detsnthresh, 0, "Minimum S/N of true pseudo-detections", 0, "ratio"); p->olabel->name = p->onlydetection ? "DETECTIONS" : "OBJECTS"; gal_fits_img_write(p->olabel, p->cp.output, keys, PROGRAM_NAME); p->olabel->name=NULL; keys=NULL; /* Write the clumps labels and useful information into it's header. Note that to make the clumps image more easily viewable, we will set all sky pixels to blank. Only clump pixels that have an overlapping object pixel will be use anyway, so the sky pixels are irrelevant. */ if(p->onlydetection==0) { p->clabel->name="CLUMPS"; gal_fits_key_list_add(&keys, GAL_TYPE_SIZE_T, "NUMLABS", 0, &p->numclumps, 0, "Total number of clumps", 0, "counter"); gal_fits_key_list_add(&keys, GAL_TYPE_FLOAT32, "CLUMPSN", 0, &p->clumpsnthresh, 0, "Minimum S/N of true clumps", 0, "ratio"); gal_fits_img_write(p->clabel, p->cp.output, keys, PROGRAM_NAME); p->clabel->name=NULL; keys=NULL; } /* Write the Sky image into the output */ if(p->sky->name) free(p->sky->name); p->sky->name="SKY"; gal_tile_full_values_write(p->sky, &p->cp.tl, 1, p->cp.output, NULL, PROGRAM_NAME); p->sky->name=NULL; /* Write the Sky standard deviation into the output. */ p->std->name="SKY_STD"; gal_fits_key_list_add(&keys, GAL_TYPE_FLOAT32, "MAXSTD", 0, &p->maxstd, 0, "Maximum raw tile standard deviation", 0, p->input->unit); gal_fits_key_list_add(&keys, GAL_TYPE_FLOAT32, "MINSTD", 0, &p->minstd, 0, "Minimum raw tile standard deviation", 0, p->input->unit); gal_fits_key_list_add(&keys, GAL_TYPE_FLOAT32, "MEDSTD", 0, &p->medstd, 0, "Median raw tile standard deviation", 0, p->input->unit); gal_tile_full_values_write(p->std, &p->cp.tl, 1, p->cp.output, keys, PROGRAM_NAME); p->std->name=NULL; } /***********************************************************************/ /************* High level function ***************/ /***********************************************************************/ void noisechisel(struct noisechiselparams *p) { /* Convolve the image. */ noisechisel_convolve(p); /* Do the initial detection. */ detection_initial(p); /* Remove false detections. */ detection(p); /* Find the Sky value and subtract it from the input and convolved images. */ noisechisel_find_sky_subtract(p); /* If the user only wanted detection, ignore the segmentation steps. */ if(p->onlydetection==0) { /* Correct the convolved image channel edges if necessary. */ noisechisel_convolve_correct_ch_edges(p); /* Do the segmentation. */ segmentation(p); } else p->numobjects=p->numdetections; /* Write the output. */ noisechisel_output(p); } �gnuastro-0.5/bin/noisechisel/detection.c������������������������������������������������������������0000644�0001750�0001750�00000105732�13216276304�015354� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <gnuastro/fits.h> #include <gnuastro/binary.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "sky.h" #include "clumps.h" #include "threshold.h" /**************************************************************** ************ Initial detection ************ ****************************************************************/ void detection_initial(struct noisechiselparams *p) { char *msg; uint8_t *b, *bf; struct timeval t0, t1; /* Get the starting time. */ if(!p->cp.quiet) { gal_timing_report(NULL, "Starting to find initial detections.", 1); gettimeofday(&t0, NULL); } /* Find and apply the threshold on the input. */ threshold_quantile_find_apply(p); if(p->detectionname) { p->binary->name="THRESHOLDED"; gal_fits_img_write(p->binary, p->detectionname, NULL, PROGRAM_NAME); p->binary->name=NULL; } /* Erode the image. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); gal_binary_erode(p->binary, p->erode, p->erodengb==4 ? 1 : 2, 1); if(!p->cp.quiet) { asprintf(&msg, "Eroded %zu time%s (%zu-connectivity).", p->erode, p->erode>1?"s":"", p->erodengb); gal_timing_report(&t1, msg, 2); free(msg); } if(p->detectionname) { p->binary->name="ERODED"; gal_fits_img_write(p->binary, p->detectionname, NULL, PROGRAM_NAME); p->binary->name=NULL; } /* Correct the no-erode values. */ bf=(b=p->binary->array)+p->binary->size; do *b = *b==THRESHOLD_NO_ERODE_VALUE ? 1 : *b; while(++b<bf); /* Do the opening. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); gal_binary_open(p->binary, p->opening, p->openingngb==4 ? 1 : 2, 1); if(!p->cp.quiet) { asprintf(&msg, "Opened (depth: %zu, %s connectivity).", p->opening, p->openingngb==4 ? "4" : "8"); gal_timing_report(&t1, msg, 2); free(msg); } /* Label the connected components. */ p->numinitialdets=gal_binary_connected_components(p->binary, &p->olabel, p->binary->ndim); if(p->detectionname) { p->olabel->name="OPENED_AND_LABELED"; gal_fits_img_write(p->olabel, p->detectionname, NULL, PROGRAM_NAME); p->olabel->name=NULL; } /* Report the ending of initial detection. */ if(!p->cp.quiet) { asprintf(&msg, "%zu initial detections found.", p->numinitialdets); gal_timing_report(&t0, msg, 1); free(msg); } } /**************************************************************** ************ Pseudo detections ************ ****************************************************************/ /* Set all the pixels we don't need to Nan. */ static void detection_pseudo_sky_or_det(struct noisechiselparams *p, uint8_t *w, int s0d1) { int32_t *l=p->olabel->array; uint8_t *b=p->binary->array, *bf=b+p->binary->size; if(s0d1) /* Set all sky regions (label equal to zero) to zero, since a blank pixel is also non-zero, we don't need to check for blanks in this case. */ do *w++ = *l++ ? *b : 0; while(++b<bf); else /* Set all detected pixels to 1. */ do { *w++ = *l ? *l==GAL_BLANK_INT32 ? GAL_BLANK_UINT8 : 1 : *b; ++l; } while(++b<bf); } /* Copy the space of this tile into the full/large array. */ static void detection_write_in_large(gal_data_t *tile, gal_data_t *copy) { uint8_t *c=copy->array; GAL_TILE_PARSE_OPERATE(tile, NULL, 0, 0, {*i=*c++;}); } /* Fill the holes and open on multiple threads to find the pseudo-detections. Ideally both these should be done immediately after each other on each large tile, but when the user wants to check the steps, we need to break out of the threads at each step. */ struct fho_params { int step; uint8_t *copyspace; gal_data_t *workbin; gal_data_t *worklab; struct noisechiselparams *p; }; static void * detection_fill_holes_open(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct fho_params *fho_prm=(struct fho_params *)(tprm->params); struct noisechiselparams *p=fho_prm->p; void *tarray; gal_data_t *tile, *copy, *tblock; size_t i, dsize[]={1,1,1,1,1,1,1,1,1,1}; /* For upto 10-Dimensions! */ /* A temporary data structure to wrap around the copy space. Note that the initially allocated space for this tile is only 1 pixel! */ copy=gal_data_alloc(NULL, GAL_TYPE_UINT8, p->input->ndim, dsize, NULL, 0, -1, NULL, NULL, NULL); free(copy->array); copy->array=&fho_prm->copyspace[p->maxltcontig*tprm->id]; /* Go over all the tiles given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* For easy reading. */ tile=&p->ltl.tiles[tprm->indexs[i]]; /* Change the tile pointers (temporarily). */ tarray=tile->array; tblock=tile->block; tile->array=gal_tile_block_relative_to_other(tile, fho_prm->workbin); tile->block=fho_prm->workbin; /* Copy the tile into the contiguous patch of memory to work on, but first reset the size element so `gal_data_copy_to_allocated' knows there is enough space. */ copy->size=p->maxltcontig; gal_data_copy_to_allocated(tile, copy); /* Fill the holes in this tile: holes with maximal connectivity means that they are most strongly bounded. */ gal_binary_fill_holes(copy, copy->ndim, -1); if(fho_prm->step==1) { detection_write_in_large(tile, copy); tile->array=tarray; tile->block=tblock; continue; } /* Open all the regions. */ gal_binary_open(copy, 1, 1, 1); /* Write the copied region back into the large input and AFTERWARDS, correct the tile's pointers, the pointers must not be corrected before writing the copy. */ detection_write_in_large(tile, copy); tile->array=tarray; tile->block=tblock; } /* Clean up. */ copy->array=NULL; gal_data_free(copy); /* Wait until all the threads finish and return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* We have the thresholded image (with blank values for regions that should not be used). Find the pseudo-detections in those regions. */ static size_t detection_pseudo_find(struct noisechiselparams *p, gal_data_t *workbin, gal_data_t *worklab, int s0d1) { gal_data_t *bin; struct fho_params fho_prm={0, NULL, workbin, worklab, p}; /* Set all the initial detected pixels to blank values. */ detection_pseudo_sky_or_det(p, workbin->array, s0d1); if(p->detectionname) { workbin->name = s0d1 ? "DTHRESH-ON-DET" : "DTHRESH-ON-SKY"; gal_fits_img_write(workbin, p->detectionname, NULL, PROGRAM_NAME); workbin->name=NULL; } /* Allocate the space necessary to work on each tile (to avoid having to allocate it it separately for each tile and within each thread. `maxltcontig' is the maximum contiguous patch of memory needed to store all tiles. Finally, since we are working on a `uint8_t' type, the size of each element is only 1 byte. */ fho_prm.copyspace=gal_data_malloc_array(GAL_TYPE_UINT8, p->cp.numthreads*p->maxltcontig, __func__, "fho_prm.copyspace"); /* Fill the holes and open on each large tile. When no check image is requested, the two steps can be done independently on each tile, but when a check image is requested, we need to break out of the thread spinning function to save the full image then continue it. */ if( p->detectionname ) { /* Necessary initializations. */ bin=gal_data_copy(workbin); /* - Temporary array for demonstration. */ fho_prm.workbin=bin; /* - To pass onto the thread. */ fho_prm.step=1; /* - So we can break out of the threads. */ /* Do each step. */ while(fho_prm.step<3) { /* Put a copy of `workbin' into `bin' for every step (only necessary for the second step and after). For the first time it was already copied.*/ if(fho_prm.step>1) memcpy(bin->array, workbin->array, workbin->size); /* Do the respective step. */ gal_threads_spin_off(detection_fill_holes_open, &fho_prm, p->ltl.tottiles, p->cp.numthreads); /* Set the extension name based on the step. */ switch(fho_prm.step) { case 1: bin->name="HOLES-FILLED"; break; case 2: bin->name="OPENED"; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so " "we can address the issue. the value %d is not " "recognized.", __func__, PACKAGE_BUGREPORT, fho_prm.step); } /* Write the temporary array into the check image. */ gal_fits_img_write(bin, p->detectionname, NULL, PROGRAM_NAME); /* Increment the step counter. */ ++fho_prm.step; } /* Clean up: the array in `bin' should just be replaced with that in `workbin' because it is used in later steps. */ if(workbin->mmapname) { /* Delete the memory mapped file and set the filename of `bin' for `workbin'. */ remove(workbin->mmapname); free(workbin->mmapname); workbin->mmapname=bin->mmapname; bin->mmapname=NULL; } else free(workbin->array); workbin->array=bin->array; bin->name=bin->array=NULL; gal_data_free(bin); } else gal_threads_spin_off(detection_fill_holes_open, &fho_prm, p->ltl.tottiles, p->cp.numthreads); /* Clean up. */ free(fho_prm.copyspace); /* Label all regions, but first, deal with the blank pixels in the `workbin' dataset when working on the Sky. Recall that in this case, the blank pixels are the detections. On the Sky image, blank should be set to 1 (because we want the detected objects to have the same labels as the pseudo-detections that cover them). This will allow us to later remove these pseudo-detections. if(s0d1==0) { bf=(b=workbin->array)+workbin->size; do if(*b==GAL_BLANK_UINT8) *b = !s0d1; while(++b<bf); } */ return gal_binary_connected_components(workbin, &worklab, 1); } /* Write the S/N tables to a file. */ static void detection_sn_write_to_file(struct noisechiselparams *p, gal_data_t *sn, gal_data_t *snind, int s0d1D2) { char *str; gal_list_str_t *comments=NULL; /* Comment for extension on further explanation. */ asprintf(&str, "See also: `%s' HDU of output with " "`--checkdetection'", ( s0d1D2<2 ? "PSEUDOS-FOR-SN": "DILATED" )); gal_list_str_add(&comments, str, 0); /* Description comment. */ str = ( s0d1D2 ? ( s0d1D2==2 ? "S/N of grown detections." : "Pseudo-detection S/N over initial detections." ) : "Pseudo-detection S/N over initial undetections."); gal_list_str_add(&comments, str, 1); /* Set the file name. */ str = ( s0d1D2 ? ( s0d1D2==2 ? p->detsn_D_name : p->detsn_d_name ) : p->detsn_s_name ); threshold_write_sn_table(p, sn, snind, str, comments); gal_list_str_free(comments, 1); /* Abort NoiseChisel if the user asked for it. */ if(s0d1D2==2 && !p->continueaftercheck) ui_abort_after_check(p, p->detsn_s_name, p->detsn_d_name, "pseudo-detection and grown/final detection S/N " "values in a table"); } static gal_data_t * detection_sn(struct noisechiselparams *p, gal_data_t *worklab, size_t num, int s0d1D2, char *extname) { float *snarr; uint8_t *flag; size_t tablen=num+1; gal_data_t *sn, *snind; int32_t *plabend, *indarr=NULL; double ave, err, *xy, *brightness; size_t ind, ndim=p->input->ndim, xyncols=1+ndim; size_t i, *area, counter=0, *dsize=p->input->dsize; float *img=p->input->array, *f=p->input->array, *ff=f+p->input->size; int32_t *plab = worklab->array, *dlab = s0d1D2 ? NULL : p->olabel->array; size_t *coord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "coord"); /* Sanity check. */ if(p->input->type!=GAL_TYPE_FLOAT32) error(EXIT_FAILURE, 0, "%s: the input dataset must be float32 type, " "it is %s", __func__, gal_type_name(p->input->type, 1)); if(!isnan(GAL_BLANK_FLOAT32)) error(EXIT_FAILURE, 0, "%s: only a NaN value is recognized for blank " "floating point data types, the blank value is defined to be %f", __func__, GAL_BLANK_FLOAT32); if(ndim!=2) error(EXIT_FAILURE, 0, "%s: only 2D datasets are acceptable, your input " "is %zu dimensions", __func__, ndim); /* Allocate all the necessary arrays, note that since we want to put each object's information into the same index, the number of allocated spaces has to be `tablen=num+1'. */ area = gal_data_calloc_array(GAL_TYPE_SIZE_T, tablen, __func__, "area"); brightness = gal_data_calloc_array(GAL_TYPE_FLOAT64, tablen, __func__, "brightness"); xy = gal_data_calloc_array(GAL_TYPE_FLOAT64, xyncols*tablen, __func__, "xy"); flag = ( s0d1D2==0 ? gal_data_calloc_array(GAL_TYPE_UINT8, tablen, __func__, "flag") : NULL ); sn = gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &tablen, NULL, 1, p->cp.minmapsize, "SIGNAL-TO-NOISE", "ratio", NULL); snind = ( p->checkdetsn==0 ? NULL : gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &tablen, NULL, 1, p->cp.minmapsize, "LABEL", "counter", NULL) ); /* Go over all the pixels and get the necessary information. */ do { /* All this work is only necessary when we are actually on a pseudo-detection label: it is non-zero and not blank. */ if(*plab && ( (p->input->flag | GAL_DATA_FLAG_HASBLANK) && *plab!=GAL_BLANK_INT32 ) ) { /* For Sky pseudo-detections we'll start to see if it has already been determined that the object lies over a detected object or not. If it does, then just ignore it. */ if(s0d1D2==0) { if( flag[*plab] ) { ++plab; ++dlab; continue; } else if(*dlab) /* We are on a detection. */ { flag[*plab]=1; area[*plab]=0; ++plab; ++dlab; continue; } } /* If we are on a blank pixel, ignore this pixel. */ if( isnan(*f) ) { ++plab; if(s0d1D2==0) ++dlab; continue; } /* Save all the necessary values. */ ++area[*plab]; brightness[*plab] += *f; if( *f > 0.0f ) /* For calculatiing the approximate center, */ { /* necessary for calculating Sky and STD. */ xy[*plab*xyncols ] += *f; xy[*plab*xyncols+1] += (double)((f-img)/dsize[1]) * *f; xy[*plab*xyncols+2] += (double)((f-img)%dsize[1]) * *f; } } /* Increment the other two labels. */ ++plab; if(s0d1D2==0) ++dlab; } while(++f<ff); /* A small sanity check. { size_t i; for(i=1;i<num+1;++i) printf("%zu (%u): %-5zu %-13.3f %-13.3f %-13.3f %-13.3f\n", i, flag[i], area[i], brightness[i], xy[i*xyncols], xy[i*xyncols+1], xy[i*xyncols+2]); } */ /* If the user wants to see the steps (on the background) and we are working on pseudo-detections, remove those that will not be used in the final quantile calculation. */ if(p->detectionname) { if(s0d1D2<2) { plabend = (plab=worklab->array) + worklab->size; do if( *plab!=GAL_BLANK_INT32 && ( area[*plab]<p->detsnminarea || brightness[*plab]<0) ) *plab=0; while(++plab<plabend); } worklab->name=extname; gal_fits_img_write(worklab, p->detectionname, NULL, PROGRAM_NAME); worklab->name=NULL; } /* Calculate the signal to noise for successful detections: */ snarr=sn->array; if(snind) indarr=snind->array; if(s0d1D2) { snarr[0]=NAN; if(snind) indarr[0]=GAL_BLANK_INT32; } for(i=1;i<tablen;++i) { ave=brightness[i]/area[i]; if( area[i]>p->detsnminarea && ave>0.0f && xy[i*xyncols]>0.0f ) { /* Get the flux weighted center coordinates. */ coord[0]=GAL_DIMENSION_FLT_TO_INT( xy[i*xyncols+1]/xy[i*xyncols] ); coord[1]=GAL_DIMENSION_FLT_TO_INT( xy[i*xyncols+2]/xy[i*xyncols] ); /* Calculate the Sky and Sky standard deviation on this tile. */ ave -= ((float *)(p->sky->array))[ gal_tile_full_id_from_coord(&p->cp.tl, coord) ]; err = ((float *)(p->std->array))[ gal_tile_full_id_from_coord(&p->cp.tl, coord) ]; /* If the image was already sky subtracted, the second power of the error needs to be doubled. */ err *= p->skysubtracted ? err : 2.0f*err; /* Correct the index in the sn to store the Signal to noise ratio. When we are dealing with the noise, we only want the non-zero signal to noise values, so we will just use a counter. But for initial detections, it is very important that their Signal to noise ratio be placed in the same index as their label. */ ind = s0d1D2 ? i : counter++; if(snind) indarr[ind]=i; snarr[ind] = ( sqrt( (float)(area[i])/p->cpscorr ) * ave / sqrt(ave+err) ); } else /* In detection pseudo-detections, order matters, so we will set all non-usable values to blank. */ if(s0d1D2) { snarr[i]=NAN; if(snind) indarr[i]=GAL_BLANK_INT32;; } } /* If we are in Sky mode, the sizes have to be corrected */ if(s0d1D2==0) { sn->dsize[0]=sn->size=counter; if(snind) snind->dsize[0]=snind->size=counter; } /* If the user wanted a list of S/N values for all pseudo-detections, save it. */ if(snind) detection_sn_write_to_file(p, sn, snind, s0d1D2); /* Clean up and return. */ free(xy); free(area); free(coord); free(brightness); if(flag) free(flag); if(snind) gal_data_free(snind); return sn; } /* ONLY FOR PSEUDO DETECTIONS: remove pseudo-detections that have a small S/N from the binary image (the labeled image will be left untouched). */ static void detection_pseudo_remove_low_sn(struct noisechiselparams *p, gal_data_t *workbin, gal_data_t *worklab, gal_data_t *sn) { size_t i; float *snarr=sn->array; uint8_t *b=workbin->array; int32_t *l=worklab->array, *lf=l+worklab->size; uint8_t *keep=gal_data_calloc_array(GAL_TYPE_UINT8, sn->size, __func__, "keep"); /* Specify the new labels for those that must be kept/changed. Note that when an object didn't have an S/N, its S/N was given a value of NaN (which will fail on any condition), so it acts as if it had an S/N lower than the required value. */ for(i=0;i<sn->size;++i) if( snarr[i] > p->detsnthresh ) keep[i]=1; /* Go over the pseudo-detection labels and only keep those that must be kept (using the new labels) in the binary array. */ if( p->input->flag & GAL_DATA_FLAG_HASBLANK ) do *b++ = *l == GAL_BLANK_INT32 ? GAL_BLANK_UINT8 : keep[ *l ] > 0; while(++l<lf); else do *b++ = keep[ *l ] > 0; while(++l<lf); /* If the user wanted to see the steps. */ if(p->detectionname) { workbin->name="TRUE-PSEUDOS"; gal_fits_img_write(workbin, p->detectionname, NULL, PROGRAM_NAME); workbin->name=NULL; } /* Clean up: */ free(keep); } /* Find and do the necessary work on pseudo-detections. */ static gal_data_t * detection_pseudo_real(struct noisechiselparams *p) { char *msg; size_t numpseudo; struct timeval t1; gal_data_t *sn, *quant, *workbin, *worklab; /* Allocate the space for the working datasets. */ worklab=gal_data_copy(p->olabel); workbin=gal_data_alloc(NULL, GAL_TYPE_UINT8, p->input->ndim, p->input->dsize, p->input->wcs, 0, p->cp.minmapsize, NULL, NULL, NULL); workbin->flag=p->input->flag; /* Over the Sky: find the pseudo-detections and make the S/N table. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); numpseudo=detection_pseudo_find(p, workbin, worklab, 0); sn=detection_sn(p, worklab, numpseudo, 0, "PSEUDOS-FOR-SN"); /* A small sanity check */ if( sn->size < p->minnumfalse) error(EXIT_FAILURE, 0, "only %zu pseudo-detections could be found over " "the sky region to estimate an S/N. This is less than %zu (value " "to `--minnumfalse' option). Please adjust parameters like " "`--dthresh', `--detsnminarea', or make sure that there actually " "is sufficient sky area after initial detection. You can use " "`--checkdetection' to see every step until this point", sn->size, p->minnumfalse); /* Get the S/N quantile and report it if we are in non-quiet mode. */ quant=gal_statistics_quantile(sn, p->detquant, 1); p->detsnthresh = *((float *)(quant->array)); if(!p->cp.quiet) { asprintf(&msg, "Pseudo-det S/N: %.2f (%.2f quant of %zu).", p->detsnthresh, p->detquant, sn->size); gal_timing_report(&t1, msg, 2); free(msg); } gal_data_free(sn); gal_data_free(quant); /* Over the detections: find pseudo-detections and make S/N table. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); numpseudo=detection_pseudo_find(p, workbin, worklab, 1); sn=detection_sn(p, worklab, numpseudo, 1, "PSEUDOS-FOR-SN"); /* Remove the pseudo detections with a low S/N. */ detection_pseudo_remove_low_sn(p, workbin, worklab, sn); /* Clean up and return. */ gal_data_free(sn); gal_data_free(worklab); return workbin; } /* This is for the final detections (grown) detections. */ static size_t detection_final_remove_small_sn(struct noisechiselparams *p, gal_data_t *workbin, size_t num) { size_t i; int8_t *b; float *snarr; gal_data_t *sn, *snind; int32_t *l, *lf, curlab=1; gal_list_str_t *comments=NULL; int32_t *newlabs=gal_data_calloc_array(GAL_TYPE_INT32, num+1, __func__, "newlabs"); /* Get the Signal to noise ratio of all detections. */ sn=detection_sn(p, p->olabel, num, 2, "DILATED"); /* Only keep the objects with an S/N above the pseudo-detection limit. */ snarr=sn->array; for(i=1;i<num+1;++i) newlabs[i] = snarr[i] > p->detsnthresh ? curlab++ : 0; /* Go over the labeled image and correct the labels. */ b=workbin->array; lf=(l=p->olabel->array)+p->olabel->size; if( p->input->flag & GAL_DATA_FLAG_HASBLANK ) { do { if( *l != GAL_BLANK_INT32 ) *b = (*l=newlabs[ *l ]) > 0; ++b; } while(++l<lf); } else do *b++ = (*l=newlabs[ *l ]) > 0; while(++l<lf); /* Save the S/N values if the user asked for them. */ if(p->detsn_D_name) { /* Make the S/N index array. */ snind=gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &num, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Fill in the indexs. Note that the S/N array had num+1 elements, so we also want to shift them back by one element, so we also need to correct its size. */ l=snind->array; sn->size = sn->dsize[0] = num; for(i=0;i<num;++i) { l[i]=i+1; snarr[i]=snarr[i+1]; } /* Make the comments, then write the table. */ gal_list_str_add(&comments, "See also: `DILATED' " "HDU of output with `--checkdetection'.", 1); gal_list_str_add(&comments, "S/N of finally grown detections.", 1); threshold_write_sn_table(p, sn, snind, p->detsn_D_name, comments); gal_list_str_free(comments, 1); } /* Clean up and return. */ free(newlabs); gal_data_free(sn); return curlab-1; } /**************************************************************** ************ Removing false detections ************ ****************************************************************/ static size_t detection_remove_false_initial(struct noisechiselparams *p, gal_data_t *workbin) { size_t i; uint8_t *b=workbin->array; int32_t *l=p->olabel->array, *lf=l+p->olabel->size, curlab=1; int32_t *newlabels=gal_data_calloc_array(GAL_TYPE_UINT32, p->numinitialdets+1, __func__, "newlabels"); /* Find the new labels for all the existing labels. Recall that `newlabels' was initialized to zero, so any label that is not given a new label here will be automatically removed. After the first pixel of a label overlaps with dbyt[i], we don't need to check the rest of that object's pixels. At this point, tokeep is only binary: 0 or 1. Note that the zeroth element of tokeep can also be non zero, this is because the holes of the labeled regions might be filled during filling the holes, but have not been filled in the original labeled array. They are not important so you can just ignore them. */ do { if( *l && *l!=GAL_BLANK_INT32 ) { newlabels[ *l ] = newlabels[ *l ] /* Have we already checked this label? */ ? 1 /* Yes we have. Just set it to 1. */ : *b; /* No we haven't, check pseudo-detection. */ } ++b; } while(++l<lf); newlabels[0]=0; /* Now that we know which labels to keep, set the new labels for the detections that must be kept. */ for(i=0;i<p->numinitialdets;++i) if(newlabels[i]) newlabels[i] = curlab++; /* Replace the byt and olab values with their proper values. If the user doesn't want to grow, then change the labels in `lab' too. Otherwise, you don't have to worry about the label array. After dilation a new labeling will be done and the whole labeled array will be re-filled.*/ b=workbin->array; l=p->olabel->array; if(p->detgrowquant==1.0f) /* We need the binary array even when */ do /* there is no growth: the binary */ { /* array is used for estimating the */ if(*l!=GAL_BLANK_INT32) /* Sky and its STD. */ *b = ( *l = newlabels[ *l ] ) > 0; ++b; } while(++l<lf); else do { if(*l!=GAL_BLANK_INT32) *b = newlabels[ *l ] > 0; ++b; } while(++l<lf); /* Clean up and return. */ free(newlabels); return curlab-1; } static size_t detection_quantile_expand(struct noisechiselparams *p, gal_data_t *workbin) { int32_t *o, *of; size_t *d, counter=0, numexpanded; float *i, *e_th, *arr=p->conv->array; gal_data_t *exp_thresh_full, *diffuseindexs; uint8_t *b=workbin->array, *bf=b+workbin->size; /* Expand the threshold values (from one value for each tile) to the whole dataset. Since we know the tiles cover the whole image, we don't neeed to initialize or check for blanks.*/ exp_thresh_full=gal_tile_block_write_const_value(p->expand_thresh, p->cp.tl.tiles, 0, 0); /* Count the pixels that must be expanded. */ e_th=exp_thresh_full->array; do { if(*b++==0 && *arr>*e_th) ++counter; ++arr; ++e_th; } while(b<bf); /* Allocate the space necessary to keep the index of all the pixels that must be expanded and re-initialize the necessary pointers. */ diffuseindexs=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 1, &counter, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Fill in the diffuse indexs and initialize the objects dataset. */ b=workbin->array; arr=p->conv->array; d=diffuseindexs->array; e_th=exp_thresh_full->array; of=(o=p->olabel->array)+p->olabel->size; do { /* If the binary value is 1, then we want an initial label of 1 (the object is already detected). If it isn't, then we only want it if it is above the threshold. */ *o = *b==1 ? 1 : ( *arr>*e_th ? CLUMPS_INIT : 0); if(*b==0 && *arr>*e_th) *d++ = o - (int32_t *)(p->olabel->array); /* Increment the points and go onto the next pixel. */ ++b; ++arr; ++e_th; } while(++o<of); /* Expand the detections. */ clumps_grow(p->olabel, diffuseindexs, 0, p->olabel->ndim); /* Only keep the 1 valued pixels in the binary array and fill its holes. */ o=p->olabel->array; bf=(b=workbin->array)+workbin->size; do *b = (*o++ == 1); while(++b<bf); workbin=gal_binary_dilate(workbin, 1, 1, 1); gal_binary_fill_holes(workbin, 1, p->detgrowmaxholesize); /* Get the labeled image. */ numexpanded=gal_binary_connected_components(workbin, &p->olabel, workbin->ndim); /* Set all the input's blank pixels to blank in the labeled and binary arrays. */ if( gal_blank_present(p->input, 1) ) { b=workbin->array; i=p->input->array; of=(o=p->olabel->array)+p->olabel->size; do { if(isnan(*i++)) { *o=GAL_BLANK_INT32; *b=GAL_BLANK_UINT8; } ++b; } while(++o<of); } /* Clean up and return */ gal_data_free(p->expand_thresh); gal_data_free(exp_thresh_full); gal_data_free(diffuseindexs); return numexpanded; } /* The initial detection has been done, now we want to remove false detections. */ void detection(struct noisechiselparams *p) { char *msg; gal_data_t *workbin; struct timeval t0, t1; size_t num_true_initial; /* Report for the user. */ if(!p->cp.quiet) { gal_timing_report(NULL, "Starting to find/remove false detections.", 1); gettimeofday(&t0, NULL); } /* Find the Sky and its Standard Deviation from the initial detectios. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); sky_and_std(p, p->detskyname); if(!p->cp.quiet) gal_timing_report(&t1, "Initial (crude) Sky and its STD found.", 2); /* Apply the sky threshold. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); threshold_apply(p, p->sky->array, p->std->array, THRESHOLD_SKY_STD); if(!p->cp.quiet) { asprintf(&msg, "Pseudo-detection thresh (%.3f sigma) applied.", p->dthresh); gal_timing_report(&t1, msg, 2); free(msg); } /* Find the real pseudo-detections. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); workbin=detection_pseudo_real(p); /* Only keep the initial detections that overlap with the real pseudo-detections. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); num_true_initial=detection_remove_false_initial(p, workbin); if(!p->cp.quiet) { asprintf(&msg, "%zu false initial detections removed.", p->numinitialdets - num_true_initial); gal_timing_report(&t1, msg, 2); free(msg); } /* If the user asked for dilation/expansion, then apply it and report the final number of detections. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); if(p->detgrowquant!=1.0f) num_true_initial=detection_quantile_expand(p, workbin); if(!p->cp.quiet) { if(p->detgrowquant==1.0f) asprintf(&msg, "%zu detections with no growth.", num_true_initial); else asprintf(&msg, "%zu detections after growth to %.3f quantile.", num_true_initial, p->detgrowquant); gal_timing_report(&t1, msg, 2); free(msg); } /* When the final (grown or over-all object) detection's S/N is less than the pseudo-detection's S/N limit, the object is false. For a real detection, the actual object S/N should be higher than any of its pseudo-detection because it has a much larger area (and possibly more flux under it). So when the final S/N is smaller than the minimum acceptable S/N threshold, we have a false pseudo-detection. */ p->numdetections = ( p->cleangrowndet ? detection_final_remove_small_sn(p, workbin, num_true_initial) : num_true_initial ); if(!p->cp.quiet) { asprintf(&msg, "%zu final true detections.", p->numdetections); gal_timing_report(&t0, msg, 1); free(msg); } if(p->detectionname) { p->olabel->name="DETECTION-FINAL"; gal_fits_img_write(p->olabel, p->detectionname, NULL, PROGRAM_NAME); p->olabel->name=NULL; } /* p->binary was used to keep the initial pseudo-detection threshold. But we don't need it any more, so we'll just free it and put the `workbin' array in its place. Note that `workbin' has a map of all the detected objects, which is still necessary during NoiseChisel. */ gal_data_free(p->binary); p->binary=workbin; /* The initial Sky and Sky STD values were only for detection. */ gal_data_free(p->sky); gal_data_free(p->std); p->sky = p->std = NULL; /* If the user wanted to check the threshold and hasn't called `continueaftercheck', then stop NoiseChisel. */ if(p->detectionname && !p->continueaftercheck) ui_abort_after_check(p, p->detectionname, NULL, "showing all detection steps"); } ��������������������������������������gnuastro-0.5/bin/noisechisel/clumps.c���������������������������������������������������������������0000644�0001750�0001750�00000163262�13216276304�014703� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <gnuastro/fits.h> #include <gnuastro/qsort.h> #include <gnuastro/blank.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "ui.h" #include "clumps.h" #include "threshold.h" /**************************************************************** ***************** Over segmentation ******************** ****************************************************************/ /* Over-segment the region specified by its indexs into peaks and their respective regions (clumps). This is very similar to the immersion method of Vincent & Soille(1991), but here, we will not separate the image into layers, instead, we will work based on the ordered flux values. If a certain pixel (at a certain level) has no neighbors, it is a local maximum and will be assigned a new label. If it has a labeled neighbor, it will take that label and if there is more than one neighboring labeled region that pixel will be a `river` pixel. */ void clumps_oversegment(struct clumps_thread_params *cltprm) { struct noisechiselparams *p=cltprm->clprm->p; size_t ndim=p->input->ndim; float *arr=p->conv->array; gal_data_t *indexs=cltprm->indexs; gal_list_sizet_t *Q=NULL, *cleanup=NULL; size_t *a, *af, ind, *dsize=p->input->dsize; size_t *dinc=gal_dimension_increment(ndim, dsize); int32_t n1, nlab, rlab, curlab=1, *clabel=p->clabel->array; /********************************************* For checks and debugging:* gal_data_t *crop; size_t extcount=1; int32_t *cr, *crf; size_t checkdsize[2]={10,10}; size_t checkstart[2]={50,145}; char *filename="clumpbuild.fits"; size_t checkstartind=gal_dimension_coord_to_index(2, dsize, checkstart); gal_data_t *tile=gal_data_alloc(gal_data_ptr_increment(arr, checkstartind, p->conv->type), GAL_TYPE_INVALID, 2, checkdsize, NULL, 0, 0, NULL, NULL, NULL); tile->block=p->conv; gal_checkset_writable_remove(filename, 0, 0); if(p->cp.numthreads!=1) error(EXIT_FAILURE, 0, "in the debugging mode of `clumps_oversegment' " "only one thread must be used"); crop=gal_data_copy(tile); gal_fits_img_write(crop, filename, NULL, PROGRAM_NAME); gal_data_free(crop); printf("blank: %u\nriver: %u\ntmpcheck: %u\ninit: %u\nmaxlab: %u\n", (int32_t)GAL_BLANK_INT32, (int32_t)CLUMPS_RIVER, (int32_t)CLUMPS_TMPCHECK, (int32_t)CLUMPS_INIT, (int32_t)CLUMPS_MAXLAB); tile->array=gal_tile_block_relative_to_other(tile, p->clabel); tile->block=p->clabel; **********************************************/ /* If the size of the indexs is zero, then this function is pointless. */ if(indexs->size==0) { cltprm->numinitclumps=0; return; } /* Sort the given indexs based on their flux (`gal_qsort_index_arr' is defined as static in `gnuastro/qsort.h') */ gal_qsort_index_arr=p->conv->array; qsort(indexs->array, indexs->size, sizeof(size_t), gal_qsort_index_float_decreasing); /* Initialize the region we want to over-segment. */ af=(a=indexs->array)+indexs->size; do clabel[*a]=CLUMPS_INIT; while(++a<af); /* Go over all the given indexs and pull out the clumps. */ af=(a=indexs->array)+indexs->size; do /* When regions of a constant flux or masked regions exist, some later indexs (although they have same flux) will be filled before hand. If they are done, there is no need to do them again. */ if(clabel[*a]==CLUMPS_INIT) { /* It might happen where one or multiple regions of the pixels under study have the same flux. So two equal valued pixels of two separate (but equal flux) regions will fall immediately after each other in the sorted list of indexs and we have to account for this. Therefore, if we see that the next pixel in the index list has the same flux as this one, it does not guarantee that it should be given the same label. Similar to the breadth first search algorithm for finding connected components, we will search all the neighbours and the neighbours of those neighbours that have the same flux of this pixel to see if they touch any label or not and to finally give them all the same label. */ if( (a+1)<af && arr[*a]==arr[*(a+1)] ) { /* Label of first neighbor found. */ n1=0; /* A small sanity check. */ if(Q!=NULL || cleanup!=NULL) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so " "we can fix this problem. `Q' and `cleanup' should be " "NULL but while checking the equal flux regions they " "aren't", __func__, PACKAGE_BUGREPORT); /* Add this pixel to a queue. */ gal_list_sizet_add(&Q, *a); gal_list_sizet_add(&cleanup, *a); clabel[*a] = CLUMPS_TMPCHECK; /* Find all the pixels that have the same flux and are connected. */ while(Q!=NULL) { /* Pop an element from the queue. */ ind=gal_list_sizet_pop(&Q); /* Look at the neighbors and see if we already have a label. */ GAL_DIMENSION_NEIGHBOR_OP(ind, ndim, dsize, ndim, dinc, { /* If it is already decided to be a river, then stop looking at the neighbors. */ if(n1!=CLUMPS_RIVER) { /* For easy reading. */ nlab=clabel[ nind ]; /* This neighbor's label isn't zero. */ if(nlab) { /* If this neighbor has not been labeled yet and has an equal flux, add it to the queue to expand the studied region.*/ if( nlab==CLUMPS_INIT && arr[nind]==arr[*a] ) { clabel[nind]=CLUMPS_TMPCHECK; gal_list_sizet_add(&Q, nind); gal_list_sizet_add(&cleanup, nind); } else n1=( nlab>0 /* If this neighbor has a positive nlab, it belongs to another object, so if `n1' has not been set for the whole region (n1==0), put `nlab' into `n1'. If `n1' has been set and is different from `nlab' then this whole equal flux region should be a wide river because it is connecting two connected regions.*/ ? ( n1 ? (n1==nlab ? n1 : CLUMPS_RIVER) : nlab ) /* If the data has blank pixels (recall that blank in int32 is negative), see if the neighbor is blank and if so, set the label to a river. Since the flag checking can be done outside this loop, for datasets with no blank element this last step will be completley ignored. */ : ( ( (p->input->flag & GAL_DATA_FLAG_HASBLANK) && nlab==GAL_BLANK_INT32 ) ? CLUMPS_RIVER : n1 ) ); } /* If this neigbour has a label of zero, then we are on the edge of the indexed region (the neighbor is not in the initial list of pixels to segment). When over-segmenting the noise and the detections, `clabel' is zero for the parts of the image that we are not interested in here. */ else clabel[*a]=CLUMPS_RIVER; } } ); } /* Set the label that is to be given to this equal flux region. If `n1' was set to any value, then that label should be used for the whole region. Otherwise, this is a new label, see the case for a non-flat region. */ if(n1) rlab = n1; else { rlab = curlab++; if( cltprm->topinds ) /* This is a local maximum of */ cltprm->topinds[rlab]=*a; /* this region, save its index.*/ } /* Give the same label to the whole connected equal flux region, except those that might have been on the side of the image and were a river pixel. */ while(cleanup!=NULL) { ind=gal_list_sizet_pop(&cleanup); /* If it was on the sides of the image, it has been changed to a river pixel. */ if( clabel[ ind ]==CLUMPS_TMPCHECK ) clabel[ ind ]=rlab; } } /* The flux of this pixel is not the same as the next sorted flux, so simply find the label for this object. */ else { /* `n1' is the label of the first labeled neighbor found, so we'll initialize it to zero. */ n1=0; /* Go over all the fully connected neighbors of this pixel and see if all the neighbors (with maximum connectivity: the number of dimensions) that have a non-macro value (less than CLUMPS_MAXLAB) belong to one label or not. If the pixel is neighboured by more than one label, set it as a river pixel. Also if it is touching a zero valued pixel (which does not belong to this object), set it as a river pixel.*/ GAL_DIMENSION_NEIGHBOR_OP(*a, ndim, dsize, ndim, dinc, { /* When `n1' has already been set as a river, there is no point in looking at the other neighbors. */ if(n1!=CLUMPS_RIVER) { /* For easy reading. */ nlab=clabel[ nind ]; /* If this neighbor is on a non-processing label, then set the first neighbor accordingly. Note that we also want the zero valued neighbors (detections if working on sky, and sky if working on detection): we want rivers between the two domains. */ n1 = ( nlab /* nlab is non-zero. */ ? ( nlab>0 /* Neighbor has a meaningful label, so check with any previously found labeled neighbors. */ ? ( n1 ? ( nlab==n1 ? n1 : CLUMPS_RIVER ) : nlab ) /* If the dataset has blank values and this neighbor is blank, then the pixel should be a river. Note that the blank checking can be optimized out, so if the input doesn't have blank values, `nlab==GAL_BLANK_INT32' will never be checked. */ : ( (p->input->flag & GAL_DATA_FLAG_HASBLANK) && nlab==GAL_BLANK_INT32 ? CLUMPS_RIVER : n1 ) ) /* `nlab==0' (the neighbor lies in the other domain (sky or detections). To avoid the different domains touching, this pixel should be a river. */ : CLUMPS_RIVER ); } }); /* Either assign a new label to this pixel, or give it the one of its neighbors. If n1 equals zero, then this is a new peak, and a new label should be created. But if n1!=0, it is either a river pixel (has more than one labeled neighbor and has been set to `CLUMPS_RIVER' before) or all its neighbors have the same label. In both such cases, rlab should be set to n1.*/ if(n1) rlab = n1; else { rlab = curlab++; if( cltprm->topinds ) cltprm->topinds[ rlab ]=*a; } /* Put the found label in the pixel. */ clabel[ *a ] = rlab; } /********************************************* For checks and debugging: if( *a / dsize[1] >= checkstart[0] && *a / dsize[1] < checkstart[0] + checkdsize[0] && *a % dsize[1] >= checkstart[1] && *a % dsize[1] < checkstart[1] + checkdsize[1] ) { printf("%zu (%zu: %zu, %zu): %u\n", ++extcount, *a, (*a%dsize[1])-checkstart[1], (*a/dsize[1])-checkstart[0], clabel[*a]); crop=gal_data_copy(tile); crf=(cr=crop->array)+crop->size; do if(*cr==CLUMPS_RIVER) *cr=0; while(++cr<crf); gal_fits_img_write(crop, filename, NULL, PROGRAM_NAME); gal_data_free(crop); } **********************************************/ } while(++a<af); /* Save the total number of clumps. */ cltprm->numinitclumps=curlab-1; /* Set all the river pixels to zero. Note that this is only necessary for the detected clumps. When finding clumps over the Sky, we will be going over the full tile and removing rivers after this function. This is because, we set the borders of the tile to a river value and didn't include them in the list of indexs. */ if(cltprm->clprm->sky0_det1) { af=(a=indexs->array)+indexs->size; do if( clabel[*a]==CLUMPS_RIVER ) clabel[*a]=CLUMPS_INIT; while(++a<af); } /********************************************* For checks and debugging: tile->array=NULL; gal_data_free(tile); printf("Total number of clumps: %u\n", curlab-1); **********************************************/ /* Clean up. */ free(dinc); } /**********************************************************************/ /***************** Grow clumps *****************/ /**********************************************************************/ /* Make the preparations for the intiial growing the clumps to identify objects: a single standard deviation for the whole object and preparing the labels (because the growth is going to happen on the `olabel' image. */ void clumps_grow_prepare_initial(struct clumps_thread_params *cltprm) { gal_data_t *indexs=cltprm->indexs; gal_data_t *input=cltprm->clprm->p->input; struct noisechiselparams *p=cltprm->clprm->p; size_t *s, *sf, *dsize=input->dsize; size_t ndiffuse=0, coord[2], *dindexs; double wcoord[2]={0.0f,0.0f}, brightness=0.0f; float glimit, *imgss=input->array, *std=p->std->array; int32_t *olabel=p->olabel->array, *clabel=p->clabel->array; /* Find the flux weighted center (meaningful only for positive valued pixels). */ sf=(s=indexs->array)+indexs->size; do if( imgss[ *s ] > 0.0f ) { brightness += imgss[ *s ]; wcoord[0] += imgss[ *s ] * (*s/dsize[1]); wcoord[1] += imgss[ *s ] * (*s%dsize[1]); } while(++s<sf); /* Calculate the center, if no pixels were positive, use the geometric center (irrespective of flux). */ if(brightness==0.0f) { sf=(s=indexs->array)+indexs->size; do { wcoord[0] += *s / dsize[1]; wcoord[1] += *s % dsize[1]; } while(++s<sf); brightness = indexs->size; } /* Convert floatint point coordinates to FITS integers. */ coord[0] = GAL_DIMENSION_FLT_TO_INT(wcoord[0]); coord[1] = GAL_DIMENSION_FLT_TO_INT(wcoord[1]); /* Find the growth limit */ cltprm->std = std[ gal_tile_full_id_from_coord(&p->cp.tl, coord) ]; glimit = p->gthresh * cltprm->std; /* Allocate space to keep the diffuse indexs over this detection. We need to keep the actual indexs since it is our only connection to the object at this stage: we are also going to re-label the pixels to grow. For most astronomical objects, the major part of the detection area is going to be diffuse flux, so we will just allocate the same size as `indexs' array (the `dsize' will be corrected after getting the exact number. */ cltprm->diffuseindexs=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 1, cltprm->indexs->dsize, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); dindexs=cltprm->diffuseindexs->array; sf=(s=indexs->array)+indexs->size; do { olabel[*s] = clabel[*s]; if( clabel[*s]==CLUMPS_INIT ) if( imgss[*s]>glimit ) dindexs[ ndiffuse++ ] = *s; } while(++s<sf); /* Correct the sizes of the `diffuseindexs' data structure. */ cltprm->diffuseindexs->size = cltprm->diffuseindexs->dsize[0] = ndiffuse; } /* Add all the remaining pixels in the detection (below the growth threshold, or those that were not touching). Note that initially `diffuseindexs' was filled with the pixels that are above the growth threshold. That was necessary for identifying the objects. Now that we have identified the objects and labeled them, we want to add the remaining diffuse pixels to it too before doing the final growth. Note that the most efficient way is just to re-fill the `diffuseindexs' array instead of adding the pixels below the threshold and sorting them afterwards.*/ void clumps_grow_prepare_final(struct clumps_thread_params *cltprm) { size_t ndiffuse=0; size_t *dindexs=cltprm->diffuseindexs->array; int32_t *olabel=cltprm->clprm->p->olabel->array; size_t *s=cltprm->indexs->array, *sf=s+cltprm->indexs->size; /* Recall that we initially allocated `diffuseindexs' to have the same size as the indexs. So there is no problem if there are more pixels in this final round compared to the initial round. */ do if( olabel[*s] < 0 ) dindexs[ ndiffuse++ ] = *s; while(++s<sf); /* Correct the sizes of the `diffuseindexs' data structure. */ cltprm->diffuseindexs->size = cltprm->diffuseindexs->dsize[0] = ndiffuse; } /* Grow the true clumps over the diffuse regions of a detection. Note that unlike before, were river pixels would get a separate label for them selves, here, they don't, they just get set back to SEGMENTINIT. This is because some of the pixels that lie immediately between two labeled regions might not be in the blankinds array (they were below the threshold). So we have to find river pixels later on, after the growth is done independently. This function is going to be used before identifying objects and also after it (to completely fill in the diffuse area). The distinguishing point between these two steps is the presence of rivers, so you can use the `withrivers' argument. Input: labels: The labels array that must be operated on. The pixels that must be "grown" must have the value `CLUMPS_INIT' (negative). diffuseindexs: The indexs of the pixels that must be grown. withrivers: as described above. connectivity: connectivity to define neighbors for growth. */ void clumps_grow(gal_data_t *labels, gal_data_t *diffuseindexs, int withrivers, int connectivity) { int searchngb; size_t *diarray=diffuseindexs->array; int32_t n1, nlab, *olabel=labels->array; size_t *s, *sf, thisround, ndiffuse=diffuseindexs->size; size_t *dinc=gal_dimension_increment(labels->ndim, labels->dsize); /* A small sanity check: */ if(labels->type!=GAL_TYPE_INT32) error(EXIT_FAILURE, 0, "%s: `labels' has to have type of int32_t", __func__); if(diffuseindexs->type!=GAL_TYPE_SIZE_T) error(EXIT_FAILURE, 0, "%s: `diffuseindexs' has to have type of size_t", __func__); /* The basic idea is this: after growing, not all the blank pixels are necessarily filled, for example the pixels might belong to two regions above the growth threshold. So the pixels in between them (which are below the threshold will not ever be able to get a label). Therefore, the safest way we can terminate the loop of growing the objects is to stop it when the number of pixels left to fill in this round (thisround) equals the number of blanks. To start the loop, we set `thisround' to one more than the number of diffuse pixels. Note that it will be corrected immediately after the loop has started, it is just important to pass the `while'. */ thisround=ndiffuse+1; while( thisround > ndiffuse ) { /* `thisround' will keep the number of pixels to be inspected in this round. `ndiffuse' will count the number of pixels left without a label by the end of this round. Since `ndiffuse' comes from the previous loop (or outside, for the first round) it has to be saved in `thisround' to begin counting a fresh. */ thisround=ndiffuse; ndiffuse=0; /* Go over all the available indexs. */ sf=(s=diffuseindexs->array)+diffuseindexs->size; do { /* We'll begin by assuming the nearest neighbor of this pixel has no label (has a value of 0). */ n1=0; /* Check the very closest neighbors of each pixel (4-connectivity in a 2D image). Note that since this macro has multiple loops within it, we can't use break. We'll use a variable instead. */ searchngb=1; GAL_DIMENSION_NEIGHBOR_OP(*s, labels->ndim, labels->dsize, connectivity, dinc, { if(searchngb) { /* For easy reading. */ nlab = olabel[nind]; /* This neighbor's label is meaningful. */ if(nlab>0) /* This is a real label. */ { if(n1) /* A prev. neighboring label has been found. */ { if( n1 != nlab ) /* Different label from */ { /* prevously found neighbor for this pixel. */ n1=CLUMPS_RIVER; searchngb=0; } } else { /* This is the first labeld neighbor found. */ n1=nlab; /* If we want to completely fill in the region (`withrivers==0'), then there is no point in looking in other neighbors, the first neighbor we find is the one we'll use. */ if(!withrivers) searchngb=0; } } } } ); /* The loop above over neighbors finishes with three possibilities: n1==0 --> No labeled neighbor was found. n1==CLUMPS_RIVER --> Connecting two labeled regions. n1>0 --> Only has one neighbouring label. The first one means that no neighbors were found and this pixel should be kept for the next loop (we'll be growing the objects pixel-layer by pixel-layer). In the other two cases, we just need to write in the value of `n1'. */ if(n1) { olabel[*s]=n1; if(withrivers && n1==CLUMPS_RIVER) /* To keep rivers in */ diarray[ ndiffuse++ ] = *s; /* the diffuse list. */ } else diarray[ ndiffuse++ ] = *s; /* Correct the size of the `diffuseindexs' dataset. */ diffuseindexs->size = diffuseindexs->dsize[0] = ndiffuse; } while(++s<sf); } /* Clean up. */ free(dinc); } /**********************************************************************/ /***************** S/N threshold *****************/ /**********************************************************************/ /* In this function we want to find the general information for each clump in an over-segmented labeled array. The signal in each clump is the average signal inside it subtracted by the average signal in the river pixels around it. So this function will go over all the pixels in the object (already found in deblendclumps()) and add them appropriately. The output is an array of size cltprm->numinitial*INFO_NCOLS. as listed below.*/ enum infocols { INFO_X, /* Flux weighted X center col, 0 by C std. */ INFO_Y, /* Flux weighted Y center col. */ INFO_NFF, /* Number of non-negative pixels (for X,Y).*/ INFO_INFLUX, /* Tatal flux within clump. */ INFO_INAREA, /* Tatal area within clump. */ INFO_RIVFLUX, /* Tatal flux within rivers around clump. */ INFO_RIVAREA, /* Tatal area within rivers around clump. */ INFO_INSTD, /* Standard deviation at clump center. */ INFO_NCOLS, /* Total number of columns. */ }; static void clumps_get_raw_info(struct clumps_thread_params *cltprm) { struct noisechiselparams *p=cltprm->clprm->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; size_t i, *a, *af, ii, coord[2]; double *row, *info=cltprm->info->array; size_t nngb=gal_dimension_num_neighbors(ndim); float *arr=p->input->array, *std=p->std->array; size_t *dinc=gal_dimension_increment(ndim, dsize); int32_t lab, nlab, *ngblabs, *clabel=p->clabel->array; /* Allocate the array to keep the neighbor labels of river pixels. */ ngblabs=gal_data_malloc_array(GAL_TYPE_INT32, nngb, __func__, "ngblabs"); /* Go over all the pixels in this region. */ af=(a=cltprm->indexs->array)+cltprm->indexs->size; do if( !isnan(arr[ *a ]) ) { /* This pixel belongs to a clump. */ if( clabel[ *a ]>0 ) { lab=clabel[*a]; ++info[ lab * INFO_NCOLS + INFO_INAREA ]; info[ lab * INFO_NCOLS + INFO_INFLUX ] += arr[*a]; if( arr[*a]>0.0f ) { info[ lab * INFO_NCOLS + INFO_NFF ] += arr[*a]; info[ lab * INFO_NCOLS + INFO_X ] += arr[*a] * (*a/dsize[1]); info[ lab * INFO_NCOLS + INFO_Y ] += arr[*a] * (*a%dsize[1]); } } /* This pixel belongs to a river (has a value of zero and isn't blank). */ else { /* We are on a river pixel. So the value of this pixel has to be added to any of the clumps in touches. But since it might touch a labeled region more than once, we use `ngblabs' to keep track of which label we have already added its value to. `ii` is the number of different labels this river pixel has already been considered for. `ngblabs' will keep the list labels. */ ii=0; memset(ngblabs, 0, nngb*sizeof *ngblabs); /* Look into the 8-connected neighbors (recall that a connectivity of `ndim' means all pixels touching it (even on one vertice). */ GAL_DIMENSION_NEIGHBOR_OP(*a, ndim, dsize, ndim, dinc, { /* This neighbor's label. */ nlab=clabel[ nind ]; /* We only want those neighbors that are not rivers (>0) or any of the flag values. */ if(nlab>0) { /* Go over all already checked labels and make sure this clump hasn't already been considered. */ for(i=0;i<ii;++i) if(ngblabs[i]==nlab) break; /* This neighbor clump hasn't been considered yet: */ if(i==ii) { ngblabs[ii++] = nlab; ++info[ nlab * INFO_NCOLS + INFO_RIVAREA ]; info[ nlab * INFO_NCOLS + INFO_RIVFLUX ] += arr[*a]; } } } ); } } while(++a<af); /* Do the final preparations. All the calculations are only necessary for the clumps that satisfy the minimum area. So there is no need to waste time on the smaller ones. */ for(lab=1; lab<=cltprm->numinitclumps; ++lab) { row = &info [ lab * INFO_NCOLS ]; if ( row[INFO_INAREA] > p->segsnminarea ) { /* Especially over the undetected regions, it might happen that none of the pixels were positive. In that case, set the total area of the clump to zero so it is no longer considered.*/ if( row[INFO_NFF]==0.0f ) row[INFO_INAREA]=0; else { coord[0]=GAL_DIMENSION_FLT_TO_INT(row[INFO_X]/row[INFO_NFF]); coord[1]=GAL_DIMENSION_FLT_TO_INT(row[INFO_Y]/row[INFO_NFF]); row[INFO_INSTD] = std[ gal_tile_full_id_from_coord(&p->cp.tl, coord) ]; /* For a check printf("---------\n"); printf("\t%f --> %zu\n", row[INFO_Y]/row[INFO_NFF], coord[1]); printf("\t%f --> %zu\n", row[INFO_X]/row[INFO_NFF], coord[0]); printf("%u: (%zu, %zu): %.3f\n", lab, coord[1]+1, coord[0]+1, row[INFO_INSTD]); */ } } } /* Clean up. */ free(dinc); free(ngblabs); } /* Make an S/N table for the clumps in a given region. */ void clumps_make_sn_table(struct clumps_thread_params *cltprm) { struct noisechiselparams *p=cltprm->clprm->p; size_t tablen=cltprm->numinitclumps+1; float *snarr; int32_t *indarr=NULL; double I, O, Ni, var, *row; int sky0_det1=cltprm->clprm->sky0_det1; size_t i, ind, counter=0, infodsize[2]={tablen, INFO_NCOLS}; /* If there were no initial clumps, then ignore this function. */ if(cltprm->numinitclumps==0) { cltprm->snind=cltprm->sn=NULL; return; } /* Allocate the arrays to keep the final S/N table (and possibly S/N index) for this object or tile. */ cltprm->sn = &cltprm->clprm->sn[ cltprm->id ]; cltprm->sn->ndim = 1; /* Depends on `cltprm->sn' */ cltprm->sn->type = GAL_TYPE_FLOAT32; cltprm->sn->dsize = gal_data_malloc_array(GAL_TYPE_SIZE_T, 1, __func__, "cltprm->sn->dsize"); cltprm->sn->array = gal_data_malloc_array(cltprm->sn->type, tablen, __func__, "cltprm->sn->array"); cltprm->sn->size = cltprm->sn->dsize[0] = tablen; /* After dsize. */ if( cltprm->clprm->snind ) { cltprm->snind = &cltprm->clprm->snind [ cltprm->id ]; cltprm->snind->ndim = 1; /* Depends on `cltprm->snind' */ cltprm->snind->type = GAL_TYPE_INT32; cltprm->snind->dsize = gal_data_malloc_array(GAL_TYPE_SIZE_T, 1, __func__, "cltprm->snind->dsize"); cltprm->snind->size = cltprm->snind->dsize[0]=tablen;/* After dsize */ cltprm->snind->array = gal_data_malloc_array(cltprm->snind->type, tablen, __func__, "cltprm->snind->array"); } else cltprm->snind=NULL; /* Allocate the array to keep the raw information of each clump. Note the `+1' in `infodsize', this is because the labels begin with 1 and we want each label to have one row on the same label.*/ cltprm->info=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 2, infodsize, NULL, 1, p->cp.minmapsize, NULL, NULL, NULL); /* First get the raw information necessary for making the S/N table. */ clumps_get_raw_info(cltprm); /* Calculate the signal to noise ratio for successful clumps */ snarr=cltprm->sn->array; if(cltprm->snind) indarr=cltprm->snind->array; for(i=1;i<tablen;++i) { /* For readability. */ row = &( ((double *)(cltprm->info->array))[ i * INFO_NCOLS ] ); Ni = row[ INFO_INAREA ]; I = row[ INFO_INFLUX ] / row[ INFO_INAREA ]; O = row[ INFO_RIVFLUX ] / row[ INFO_RIVAREA ]; /* If the inner flux is smaller than the outer flux (happens only in noise cases) or the area is smaller than the minimum area to calculate signal-to-noise, then set the S/N of this segment to zero. */ if( I>O && Ni>p->segsnminarea ) { /* Here we have done sky subtraction once. However, if the sky was already subtracted (informed by the user), then the varience should be multiplied by 2. */ var = ( (p->skysubtracted ? 2.0f : 1.0f) * row[INFO_INSTD] * row[INFO_INSTD] ); /* Calculate the Signal to noise ratio, if we are on the noise regions, we don't care about the IDs of the clumps anymore, so store the Signal to noise ratios contiguously (for easy sorting and etc). Note that counter will always be smaller and equal to i. */ ind = sky0_det1 ? i : counter++; if(cltprm->snind) indarr[ind]=i; snarr[ind]=( sqrt(Ni/p->cpscorr) * (I-O) / sqrt( (I>0?I:-1*I) + (O>0?O:-1*O) + var ) ); } else { /* Only over detections, we should put a NaN when the S/N */ if(sky0_det1) { snarr[i]=NAN; if(cltprm->snind) indarr[i]=i; } } } /* If we are in Sky mode, the sizes have to be corrected */ if(sky0_det1==0) { cltprm->sn->dsize[0] = cltprm->sn->size = counter; if(cltprm->snind) cltprm->snind->dsize[0] = cltprm->snind->size=counter; } /* Clean up. */ gal_data_free(cltprm->info); } /* Correct the labels of the clumps that will be used in determining the S/N threshold for true clumps. */ static void clumps_correct_sky_labels_for_check(struct clumps_thread_params *cltprm, gal_data_t *tile) { gal_data_t *newinds; int32_t *ninds, curlab, *l, *lf; size_t len=cltprm->numinitclumps+1; struct noisechiselparams *p=cltprm->clprm->p; /* If there are no clumps in this tile, then this function can be ignored. */ if(cltprm->snind->size==0) return; /* A small sanity check. */ if(gal_tile_block(tile)!=p->clabel) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to address " "the problem. `tile->block' must point to the `clabel' dataset", __func__, PACKAGE_BUGREPORT); /* Allocate a dataset with the new indexs, note that it will need to have one element for each initial label (the excluded clumps need to be set to zero). So we also need to clear the allocated space. */ newinds=gal_data_alloc(NULL, p->clabel->type, 1, &len, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Get the next available label for these clumps. If more than one thread was used, we are first going to lock the mutex (so no other thread changes these values), we will then read the shared number for this thread to use, then update the shared number and finally, unlock the mutex so other threads can do the same when they get to this point. */ if(p->cp.numthreads>1) pthread_mutex_lock(&cltprm->clprm->labmutex); curlab = p->numclumps+1; /* Note that counting begins from 1. */ p->numclumps += cltprm->snind->size; if(p->cp.numthreads>1) pthread_mutex_unlock(&cltprm->clprm->labmutex); /* Initialize the newinds array to CLUMPS_INIT (which be used as a new label for all the clumps that must be removed. */ lf = (l=newinds->array) + newinds->size; do *l++=CLUMPS_INIT; while(l<lf); /* The new indexs array has been initialized to zero. So we just need to go over the labels in `cltprm->sninds' and give them a value of `curlab++'. */ ninds=newinds->array; lf = (l=cltprm->snind->array) + cltprm->snind->size; do { ninds[*l]=curlab++; *l=ninds[*l]; } while(++l<lf); /* Go over this tile and correct the values. */ GAL_TILE_PARSE_OPERATE( tile, NULL, 0, 1, {if(*i>0) *i=ninds[ *(int32_t *)i ];} ); /* Clean up. */ gal_data_free(newinds); } static void * clumps_find_make_sn_table(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct clumps_params *clprm=(struct clumps_params *)(tprm->params); struct noisechiselparams *p=clprm->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; void *tarray; double numdet; gal_data_t *tile, *tblock, *tmp; uint8_t *binary=p->binary->array; struct clumps_thread_params cltprm; size_t i, c, ind, tind, num, numsky, *indarr; size_t *scoord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "scoord"); size_t *icoord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "icoord"); /* Initialize the parameters for this thread. */ cltprm.clprm = clprm; cltprm.topinds = NULL; /* Go over all the tiles/detections given to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* IDs. */ cltprm.id = tind = tprm->indexs[i]; tile = &p->ltl.tiles[tind]; /* Change the tile's pointers to the binary image (which has 1 for detected pixels and 0 for un-detected regions). */ tarray=tile->array; tblock=tile->block; tile->array = gal_tile_block_relative_to_other(tile, p->binary); tile->block = p->binary; /* Get the number of usable elements in this tile (note that tiles can have blank pixels), so we can't simply use `tile->size'. */ if(tile->flag & GAL_DATA_FLAG_HASBLANK) { tmp=gal_statistics_number(tile); num=*((size_t *)(tmp->array)); gal_data_free(tmp); } else num=tile->size; /* Find the number of detected pixels over this tile. Since this is the binary image, this is just the sum of all the pixels. Note that `numdet' can be `nan' when the whole tile is blank and so there was no values to sum. Recall that in summing, when there is not input, the output is `nan'. */ tmp=gal_statistics_sum(tile); numdet=*((double *)(tmp->array)); gal_data_free(tmp); /* See if this tile should be used or not (has enough undetected pixels). Note that it might happen that some tiles are fully blank. In such cases, it is important to first check the number of detected pixels. */ numsky=num-numdet; if( num && (float)numsky/(float)num > p->minskyfrac ) { /* Add the indexs of all undetected pixels in this tile into an array. */ cltprm.indexs=gal_data_alloc(NULL, GAL_TYPE_SIZE_T, 1, &numsky, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Change the tile's block to the clump labels dataset (because we'll need to set the labels of the rivers on the edge of the tile here). */ tile->array = gal_tile_block_relative_to_other(tile, p->clabel); tile->block = p->clabel; /* We need to set all the pixels on the edge of the tile to rivers and not include them in the list of indexs to set clumps. To do that, we need this tile's starting coordinates. */ gal_dimension_index_to_coord(gal_data_ptr_dist(p->clabel->array, tile->array, p->clabel->type), ndim, dsize, scoord); /* Add the index of every sky element to the array of indexs. Note that since we know the array is always of type `int32_t', we can call the `GAL_TILE_PO_OISET' macro to avoid having to deal with multiple possible types in `GAL_TILE_PARSE_OPERATE'. Since the OUT macro-variable is NULL, the `int' is just a place-holder, it will not be used. */ c=0; indarr=cltprm.indexs->array; GAL_TILE_PO_OISET(int32_t, int, tile, NULL, 0, 1, { /* This pixel's index over all the image. */ ind = (int32_t *)i - (int32_t *)(p->clabel->array); gal_dimension_index_to_coord(ind, ndim, dsize, icoord); /* If the pixel is on the tile edge, set it as river and don't include it in the indexs. */ if( icoord[0]==scoord[0] || icoord[0]==scoord[0]+tile->dsize[0]-1 || icoord[1]==scoord[1] || icoord[1]==scoord[1]+tile->dsize[1]-1 ) *(int32_t *)i=CLUMPS_RIVER; /* This pixel is not on the edge, check if it had a value of `0' in the binary image (is not detected) then add it to the list of indexs (note that the binary image also contains the blank pixels, so only sky regions have a value of 0 in the binary image). */ else if( binary[ind]==0 ) { /* if(c!=cltprm.indexs->size) { if(cltprm.id==282) *i+=2; */ indarr[c++]=gal_data_ptr_dist(p->clabel->array, i, p->clabel->type); /* } else if(cltprm.id==282) { int32_t *clabel=p->clabel->array; size_t kjd=gal_data_ptr_dist(p->clabel->array, i, p->clabel->type); printf("%zu, %zu: %u\n", kjd%dsize[1]+1, kjd/dsize[1]+1, clabel[kjd]); } */ } }); /* Correct the number of indexs. */ cltprm.indexs->size=cltprm.indexs->dsize[0]=c; /* Generate the clumps over this region. */ clumps_oversegment(&cltprm); /* Set all river pixels to CLUMPS_INIT (to be distinguishable from the detected regions). */ GAL_TILE_PO_OISET( int32_t, int, tile, NULL, 0, 1, {if(*i==CLUMPS_RIVER) *i=CLUMPS_INIT;} ); /* For a check, the step variable will be set. */ if(clprm->step==1) { gal_data_free(cltprm.indexs); continue; } /* Make the clump S/N table. */ clumps_make_sn_table(&cltprm); /* If the user wanted to check the steps, remove the clumps that weren't used from the `clabel' image (they have been already excluded from the table). */ if(cltprm.snind) clumps_correct_sky_labels_for_check(&cltprm, tile); /* Clean up. */ gal_data_free(cltprm.indexs); } /* Reset the tile's pointers back to what they were. */ tile->array=tarray; tile->block=tblock; } /* Clean up. */ free(scoord); free(icoord); /* Wait for the all the threads to finish and return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /* Find the true clump signal to noise value from the clumps in the sky region. Each thread will find the useful signal to noise values for the tiles that have been assigned to it. It will then store the pointer to the S/N table into the sntablearr array (with the size of the number of meshs). If no clumps could be found in a mesh, then sntablearr[i]=NULL. Otherwise, it points to an array of the useful S/N values in that clump. Note that we don't care about the order of S/N values any more! There is also an accompanying array to keep the number of elements in the final S/N array of each mesh: numclumpsarr. Using these two arrays, after all the threads are finished, we can concatenate all the S/N values into one array and send it to the main findsnthresh function in thresh.c. */ void clumps_true_find_sn_thresh(struct noisechiselparams *p) { char *msg; struct timeval t1; size_t i, j, c, numsn=0; struct clumps_params clprm; gal_list_str_t *comments=NULL; gal_data_t *sn, *snind, *quant, *claborig; /* Get starting time for later reporting if necessary. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); /* Initialize/allocate the clump parameters structure, Note that the S/N indexs are also needed when we want to check the segmentation steps (they are used to correct the indexs in the final output). */ clprm.p=p; clprm.sky0_det1=0; clprm.sn=gal_data_array_calloc(p->ltl.tottiles); clprm.snind = ( p->checksegmentation || p->checkclumpsn ? gal_data_array_calloc(p->ltl.tottiles) : NULL ); /* If the user wants to check the steps of get an S/N table, then we need a unique label for each clump. But in each region, the labels start from 1. So we need a central place to keep the next available label. Since `p->numclumps' is not used yet, we will use it here. When multiple threads are used, we will need a mutex to make sure that only one thread can change this central variable at every one moment. */ if(p->checksegmentation || p->checkclumpsn) { p->numclumps=0; if( p->cp.numthreads > 1 ) pthread_mutex_init(&clprm.labmutex, NULL); } /* Spin off the threads to start the work. Note that several steps are done on each tile within a thread. So if the user wants to check steps, we need to break out of the processing get an over-all output, then reset the input and call it again. So it will be slower, but its is natural, since the user is testing to find the correct combination of parameters for later use. */ if(p->segmentationname) { /* Necessary initializations. */ clprm.step=1; claborig=p->clabel; p->clabel=gal_data_copy(claborig); /* Do each step. */ while(clprm.step<3) { /* Reset the temporary copy of clabel back to its original. */ if(clprm.step>1) memcpy(p->clabel->array, claborig->array, claborig->size*gal_type_sizeof(claborig->type)); /* Do this step. */ gal_threads_spin_off(clumps_find_make_sn_table, &clprm, p->ltl.tottiles, p->cp.numthreads); /* Set the extension name. */ switch(clprm.step) { case 1: p->clabel->name = "SKY_CLUMPS_ALL"; break; case 2: p->clabel->name = "SKY_CLUMPS_FOR_SN"; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so " "we can address the issue. The value %d is not valid for " "clprm.step", __func__, PACKAGE_BUGREPORT, clprm.step); } /* Write the demonstration array into the check image. The default values are hard to view, so we'll make a copy of the demo, set all Sky regions to blank and all clump macro values to zero. */ gal_fits_img_write(p->clabel, p->segmentationname, NULL, PROGRAM_NAME); /* Increment the step counter. */ ++clprm.step; } /* Clean up (we don't need the original any more). */ gal_data_free(claborig); p->clabel->name=NULL; } else { clprm.step=0; gal_threads_spin_off(clumps_find_make_sn_table, &clprm, p->ltl.tottiles, p->cp.numthreads); } /* Destroy the mutex if it was initialized. */ if( p->cp.numthreads>1 && (p->checksegmentation || p->checkclumpsn) ) pthread_mutex_destroy(&clprm.labmutex); /* Find the total number of S/N values we have for all the clumps. */ for(i=0;i<p->ltl.tottiles;++i) if(clprm.sn[i].ndim) /* Only on tiles were an S/N was calculated. */ numsn+=clprm.sn[i].size; if( numsn < p->minnumfalse ) error(EXIT_FAILURE, 0, "only %zu clumps could be identified in the " "undetected regions. This is less than %zu (value to " "`--minnumfalse' option). Please either decrease this value or " "other options to change prior processing steps", numsn, p->minnumfalse); /* Allocate the space to keep all the S/N values. */ sn=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &numsn, NULL, 0, p->cp.minmapsize, "CLUMP_S/N", "ratio", "Signal-to-noise ratio"); snind = ( p->checkclumpsn ? gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &numsn, NULL, 0, p->cp.minmapsize, "CLUMP_ID", "counter", "Unique ID for this clump.") : NULL ); /* Copy the S/N values of all the clumps into the unified array. */ c=0; for(i=0;i<p->ltl.tottiles;++i) if(clprm.sn[i].ndim) for(j=0;j<clprm.sn[i].size;++j) { ((float *)(sn->array))[c] = ((float *)(clprm.sn[i].array))[j]; if(snind) ((int32_t *)(snind->array))[c] = ((int32_t *)(clprm.snind[i].array))[j]; ++c; } /* The S/N array of sky clumps is desiged to have no blank values, so set the flags accordingly to avoid a redundant blank search. */ sn->flag = GAL_DATA_FLAG_BLANK_CH | GAL_DATA_FLAG_HASBLANK; /* If the user wanted to see the S/N table, then save it. */ if(p->checkclumpsn) { /* Make the comments, then write the table and free the comments. */ if(p->cp.numthreads>1) gal_list_str_add(&comments, "NOTE: In multi-threaded mode, clump " "IDs differ in each run and are not sorted.", 1); gal_list_str_add(&comments, "See also: `SKY_CLUMPS_FOR_SN' HDU of " "output with `--checksegmentation'.", 1); gal_list_str_add(&comments, "S/N of clumps over undetected regions.", 1); threshold_write_sn_table(p, sn, snind, p->clumpsn_s_name, comments); gal_list_str_free(comments, 1); } /* Find the desired quantile from the full S/N distribution. */ quant = gal_statistics_quantile(sn, p->segquant, 1); p->clumpsnthresh = *((float *)(quant->array)); if(!p->cp.quiet) { asprintf(&msg, "Clump S/N: %.2f (%.3f quant of %zu).", p->clumpsnthresh, p->segquant, sn->size); gal_timing_report(&t1, msg, 2); free(msg); } /* Clean up. */ gal_data_free(sn); gal_data_free(snind); gal_data_free(quant); gal_data_array_free(clprm.sn, p->ltl.tottiles, 1); gal_data_array_free(clprm.snind, p->ltl.tottiles, 1); } /***********************************************************************/ /***************** Over detections *****************/ /***********************************************************************/ /* Put the indexs of each labeled region into an array of `gal_data_t's (where each element is a dataset containing the respective label's indexs). */ gal_data_t * clumps_det_label_indexs(struct noisechiselparams *p) { size_t i, *areas; int32_t *a, *l, *lf; gal_data_t *labindexs=gal_data_array_calloc(p->numdetections+1); /* Find the area in each detected objects (to see how much space we need to allocate). */ areas=gal_data_calloc_array(GAL_TYPE_SIZE_T, p->numdetections+1, __func__, "areas"); if(gal_blank_present(p->input, 1)) { lf=(l=p->olabel->array)+p->olabel->size; /* Blank pixels have a */ do if(*l>0) ++areas[*l]; while(++l<lf); /* negative value in int32. */ } else { lf=(l=p->olabel->array)+p->olabel->size; do ++areas[*l]; while(++l<lf); areas[0]=0; } /* For a check. for(i=0;i<p->numdetections+1;++i) printf("detection %zu: %zu\n", i, areas[i]); exit(0); */ /* Allocate/Initialize the dataset containing the indexs of each object. We don't want the labels of the non-detected regions (areas[0]). So we'll set that to zero.*/ for(i=1;i<p->numdetections+1;++i) gal_data_initialize(&labindexs[i], NULL, GAL_TYPE_SIZE_T, 1, &areas[i], NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Put the indexs into each dataset. We will use the areas array again, but this time, use it as a counter. */ memset(areas, 0, (p->numdetections+1)*sizeof *areas); lf=(a=l=p->olabel->array)+p->olabel->size; do if(*l>0) /* No undetected regions (*l==0), or blank (<0) */ ((size_t *)(labindexs[*l].array))[ areas[*l]++ ] = l-a; while(++l<lf); /* Clean up and return. */ free(areas); return labindexs; } /* Only keep true clumps over detections. */ void clumps_det_keep_true_relabel(struct clumps_thread_params *cltprm) { struct noisechiselparams *p=cltprm->clprm->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; int istouching; size_t i, *s, *sf, *dinc; float *sn = cltprm->sn ? cltprm->sn->array : NULL; int32_t *l, *lf, *newlabs, curlab=1, *clabel=p->clabel->array; /* If there were no clumps over the detection, then just set the number of true clumps to zero, otherwise, see which ones should be removed. */ if(cltprm->sn) { /* Allocate the necessary arrays. */ newlabs=gal_data_malloc_array(GAL_TYPE_INT32, cltprm->numinitclumps+1, __func__, "newlabs"); dinc=gal_dimension_increment(ndim, dsize); /* Initialize the new labels with CLUMPS_INIT (so the diffuse area can be distinguished from the clumps). */ lf=(l=newlabs)+cltprm->numinitclumps+1; do *l++=CLUMPS_INIT; while(l<lf); /* Set the new labels. Here we will also be removing clumps with a peak that touches a river pixel. */ if(p->keepmaxnearriver) { for(i=1;i<cltprm->numinitclumps+1;++i) if( sn[i] > p->clumpsnthresh ) newlabs[i]=curlab++; } else { for(i=1;i<cltprm->numinitclumps+1;++i) { /* Check if all the neighbors of this top element are touching a river or not. */ istouching=0; GAL_DIMENSION_NEIGHBOR_OP(cltprm->topinds[i], ndim, dsize, ndim, dinc, { if(clabel[nind]==0) istouching=1; }); /* If the peak isn't touching a river, then check its S/N and if that is also good, give it a new label. */ if( !istouching && sn[i] > p->clumpsnthresh ) newlabs[i]=curlab++; } } /* Correct the clump labels. Note that the non-clumpy regions over the detections (rivers) have already been initialized to CLUMPS_INIT (which is negative). So we'll just need to correct the ones with a value larger than 0. */ sf=(s=cltprm->indexs->array)+cltprm->indexs->size; do if(clabel[*s]>0) clabel[*s] = newlabs[ clabel[*s] ]; while(++s<sf); /* Save the total number of true clumps in this detection. */ cltprm->numtrueclumps=curlab-1; /* Clean up. */ free(dinc); free(newlabs); } else cltprm->numtrueclumps=0; } ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/ui.c�������������������������������������������������������������������0000644�0001750�0001750�00000063101�13216276304�014004� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" Detects and segments signal " "that is deeply burried in noise. It employs a noise-based detection and " "segmentation method enabling it to be very resilient to the rich diversity " "of shapes in astronomical targets.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct noisechiselparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->numthreads = gal_threads_number(); cp->coptions = gal_commonopts_options; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: cp->coptions[i].flags=OPTION_HIDDEN; break; case GAL_OPTIONS_KEY_TILESIZE: case GAL_OPTIONS_KEY_MINMAPSIZE: case GAL_OPTIONS_KEY_NUMCHANNELS: case GAL_OPTIONS_KEY_INTERPNUMNGB: case GAL_OPTIONS_KEY_REMAINDERFRAC: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; cp->coptions[i].doc="`txt', `fits-ascii', `fits-binary'."; break; } } } /* Parse a single option: */ static error_t parse_opt(int key, char *arg, struct argp_state *state) { struct noisechiselparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->inputname) argp_error(state, "only one argument (input file) should be given"); else p->inputname=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct noisechiselparams *p) { /* If the convolved option is given, then the convolved HDU is also mandatory. */ if(p->convolvedname && p->convolvedhdu==NULL) error(EXIT_FAILURE, 0, "no value given to `--convolvedhdu'. When the " "`--convolved' option is called (to specify a convolved image " "and avoid convolution) it is mandatory to also specify a HDU " "for it"); /* Make sure the connectivities have the correct values. */ if(p->erodengb!=4 && p->erodengb!=8) error(EXIT_FAILURE, 0, "%zu not acceptable for `--erodengb'. It must " "be 4 or 8 (specifying the type of connectivity)", p->erodengb); if(p->openingngb!=4 && p->openingngb!=8) error(EXIT_FAILURE, 0, "%zu not acceptable for `--openingngb'. It must " "be 4 or 8 (specifying the type of connectivity)", p->openingngb); /* Make sure that the no-erode-quantile is not smaller or equal to qthresh. */ if( p->noerodequant <= p->qthresh) error(EXIT_FAILURE, 0, "the quantile for no erosion (`--noerodequant') " "must be larger than the base quantile threshold (`--qthresh', " "or `-t'). You have provided %.4f and %.4f for the former and " "latter, respectively", p->noerodequant, p->qthresh); /* For the options that make tables, the table formation option is mandatory. */ if( (p->checkdetsn || p->checkclumpsn) && p->cp.tableformat==0 ) error(EXIT_FAILURE, 0, "`--tableformat' is necessary with the " "`--checkdetsn' and `--checkclumpsn' options.\n" "Please see description for `--tableformat' after running the " "following command for more information (use `SPACE' to go down " "the page and `q' to return to the command-line):\n\n" " $ info gnuastro \"Input Output options\""); /* Kernel checks. */ if(p->kernelname) { /* Check if it exists. */ gal_checkset_check_file(p->kernelname); /* If its FITS, see if a HDU has been provided. */ if( gal_fits_name_is_fits(p->kernelname) && p->khdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified for kernel. When the " "kernel is a FITS file, a HDU must also be specified. You " "can use the `--khdu' option and give it the HDU number " "(starting from zero), extension name, or anything " "acceptable by CFITSIO"); } /* Wide kernel checks. */ if(p->widekernelname) { /* Check if it exists. */ gal_checkset_check_file(p->widekernelname); /* If its FITS, see if a HDU has been provided. */ if( gal_fits_name_is_fits(p->widekernelname) && p->wkhdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified for wide kernel. When the " "wide kernel is a FITS file, a HDU must also be specified. You " "can use the `--khdu' option and give it the HDU number " "(starting from zero), extension name, or anything " "acceptable by CFITSIO"); } } static void ui_check_options_and_arguments(struct noisechiselparams *p) { /* Basic input file checks. */ if(p->inputname) { /* Check if it exists. */ gal_checkset_check_file(p->inputname); /* If its FITS, see if a HDU has been provided. */ if( gal_fits_name_is_fits(p->inputname) && p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified for input. When the input " "is a FITS file, a HDU must also be specified, you can use " "the `--hdu' (`-h') option and give it the HDU number " "(starting from zero), extension name, or anything " "acceptable by CFITSIO"); } else error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ static void ui_set_output_names(struct noisechiselparams *p) { char *output=p->cp.output; char *basename = output ? output : p->inputname; /* Main program output. */ if(output) { /* Delete the file if it already exists. */ gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); /* When the output name is given (possibly with directory information), the check images will also be put in that same directory.. */ p->cp.keepinputdir=1; } else p->cp.output=gal_checkset_automatic_output(&p->cp, p->inputname, "_labeled.fits"); /* Tile check. */ if(p->cp.tl.checktiles) p->cp.tl.tilecheckname=gal_checkset_automatic_output(&p->cp, basename, "_tiles.fits"); /* Quantile threshold. */ if(p->checkqthresh) p->qthreshname=gal_checkset_automatic_output(&p->cp, basename, "_qthresh.fits"); /* Initial detection Sky values. */ if(p->checkdetsky) p->detskyname=gal_checkset_automatic_output(&p->cp, basename, "_detsky.fits"); /* Pseudo-detection S/N values. */ if(p->checkdetsn) { p->detsn_s_name=gal_checkset_automatic_output(&p->cp, basename, ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "_detsn_sky.txt" : "_detsn_sky.fits") ); p->detsn_d_name=gal_checkset_automatic_output(&p->cp, basename, ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "_detsn_det.txt" : "_detsn_det.fits") ); p->detsn_D_name=gal_checkset_automatic_output(&p->cp, basename, ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "_detsn_grown.txt" : "_detsn_grown.fits") ); } /* Detection steps. */ if(p->checkdetection) p->detectionname=gal_checkset_automatic_output(&p->cp, basename, "_det.fits"); /* Detection steps. */ if(p->checksky) p->skyname=gal_checkset_automatic_output(&p->cp, basename, "_sky.fits"); /* Clump S/N values. */ if(p->checkclumpsn) { p->clumpsn_s_name=gal_checkset_automatic_output(&p->cp, basename, ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "_clumpsn_sky.txt" : "_clumpsn_sky.fits") ); p->clumpsn_d_name=gal_checkset_automatic_output(&p->cp, basename, ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "_clumpsn_det.txt" : "_clumpsn_det.fits") ); } /* Segmentation steps. */ if(p->checksegmentation) p->segmentationname=gal_checkset_automatic_output(&p->cp, basename, "_seg.fits"); } static void ui_prepare_kernel(struct noisechiselparams *p) { /* The default kernel. It was created by saving the following commands in a script and running it. It will create a plain text array along with a FITS image. The crop is because the first and last rows and columns of all PSFs made by MakeProfiles are blank (zero) when you run with oversample=1. You can keep the spaces when copying and pasting ;-). Just make it executable and run it. set -o errexit # Stop if a program returns false. echo "0 0.0 0.0 3 2 0 0 1 1 5" > tmp.txt export GSL_RNG_TYPE=ranlxs2 export GSL_RNG_SEED=1 astmkprof tmp.txt --oversample=1 --envseed --numrandom=10000 \ --tolerance=0.01 --nomerged astcrop 0_tmp.fits --section=2:*-1,2:*-1 --zeroisnotblank \ --output=fwhm2.fits astconvertt fwhm2.fits --output=fwhm2.txt rm 0_tmp.fits tmp.txt */ size_t kernel_2d_dsize[2]={11,11}; float *f, *ff, *k, kernel_2d[121]= { 0, 0, 0, 0, 0, 6.57699e-09, 0, 0, 0, 0, 0, 0, 0, 6.57699e-09, 2.10464e-07, 1.68371e-06, 3.36742e-06, 1.68371e-06, 2.10464e-07, 6.57699e-09, 0, 0, 0, 6.57699e-09, 8.41855e-07, 2.69394e-05, 0.000383569, 0.000717224, 0.000379782, 2.69394e-05, 8.41855e-07, 6.57699e-09, 0, 0, 2.10464e-07, 2.69394e-05, 0.00140714, 0.00888549, 0.016448, 0.00867408, 0.00138203, 2.69394e-05, 2.10464e-07, 0, 0, 1.68371e-06, 0.000381138, 0.00875434, 0.0573377, 0.106308, 0.0570693, 0.00891745, 0.000378914, 1.68371e-06, 0, 6.57699e-09, 3.36742e-06, 0.00071364, 0.0164971, 0.106865, 0.197316, 0.106787, 0.0166434, 0.000713827, 3.36742e-06, 6.57699e-09, 0, 1.68371e-06, 0.000215515, 0.00894112, 0.0573699, 0.106239, 0.0567907, 0.00901191, 0.000215515, 1.68371e-06, 0, 0, 2.10464e-07, 2.69394e-05, 0.00135085, 0.0089288, 0.0164171, 0.00879334, 0.0013622, 2.69394e-05, 2.10464e-07, 0, 0, 6.57699e-09, 8.41855e-07, 2.69394e-05, 0.000215515, 0.000724137, 0.000215515, 2.69394e-05, 8.41855e-07, 6.57699e-09, 0, 0, 0, 6.57699e-09, 2.10464e-07, 1.68371e-06, 3.36742e-06, 1.68371e-06, 2.10464e-07, 6.57699e-09, 0, 0, 0, 0, 0, 0, 0, 6.57699e-09, 0, 0, 0, 0, 0 }; /* If a kernel file is given, then use it. Otherwise, use the default kernel. */ if(p->kernelname) p->kernel=gal_fits_img_read_kernel(p->kernelname, p->khdu, p->cp.minmapsize); else { /* Allocate space for the kernel (we don't want to use the statically allocated array. */ p->kernel=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 2, kernel_2d_dsize, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* Now copy the staticly allocated array into it. */ k=p->kernel->array; ff=(f=kernel_2d)+gal_dimension_total_size(2, p->kernel->dsize); do *k++=*f; while(++f<ff); } /* If a wide kernel is given, then read it into memory. Otherwise, just ignore it. */ if(p->widekernelname) p->widekernel=gal_fits_img_read_kernel(p->widekernelname, p->wkhdu, p->cp.minmapsize); } static void ui_prepare_tiles(struct noisechiselparams *p) { gal_data_t *check; struct gal_tile_two_layer_params *tl=&p->cp.tl, *ltl=&p->ltl; /* Check the tile parameters for the small tile sizes and make the tile structure. We will also need the dimensions of the tile with the maximum required memory. */ p->maxtsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, p->input->ndim, __func__, "p->maxtsize"); gal_tile_full_sanity_check(p->inputname, p->cp.hdu, p->input, tl); gal_tile_full_two_layers(p->input, tl); gal_tile_full_permutation(tl); for(check=tl->tiles; check!=NULL; check=check->next) if( check->size > p->maxtcontig )/* p->maxtcontig initialized to 0. */ { p->maxtcontig=check->size; memcpy(p->maxtsize, check->dsize, tl->ndim*sizeof *p->maxtsize); } /* Make the large tessellation, except for the size, the rest of the parameters are the same as the small tile sizes. */ ltl->numchannels = tl->numchannels; ltl->remainderfrac = tl->remainderfrac; ltl->workoverch = tl->workoverch; ltl->checktiles = tl->checktiles; ltl->oneelempertile = tl->oneelempertile; p->maxltsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, p->input->ndim, __func__, "p->maxltsize"); gal_tile_full_sanity_check(p->inputname, p->cp.hdu, p->input, ltl); gal_tile_full_two_layers(p->input, ltl); gal_tile_full_permutation(ltl); for(check=ltl->tiles; check!=NULL; check=check->next) if( check->size > p->maxltcontig )/* p->maxltcontig initialized to 0. */ { p->maxltcontig=check->size; memcpy(p->maxltsize, check->dsize, ltl->ndim*sizeof *p->maxltsize); } /* If the input has blank elements, then set teh appropriate flag for each tile.*/ if( p->input->flag & GAL_DATA_FLAG_HASBLANK ) { gal_tile_block_blank_flag(tl->tiles, p->cp.numthreads); gal_tile_block_blank_flag(ltl->tiles, p->cp.numthreads); } /* Make the tile check image if requested. */ if(tl->checktiles) { /* Large tiles. */ check=gal_tile_block_check_tiles(ltl->tiles); gal_fits_img_write(check, tl->tilecheckname, NULL, PROGRAM_NAME); gal_data_free(check); /* Small tiles. */ check=gal_tile_block_check_tiles(tl->tiles); gal_fits_img_write(check, tl->tilecheckname, NULL, PROGRAM_NAME); gal_data_free(check); /* If `continueaftercheck' hasn't been called, abort NoiseChisel. */ if(!p->continueaftercheck) ui_abort_after_check(p, tl->tilecheckname, NULL, "showing all tiles over the image"); /* Free the name. */ free(tl->tilecheckname); } } static void ui_preparations(struct noisechiselparams *p) { /* Prepare the names of the outputs. */ ui_set_output_names(p); /* Read the input as a single precision floating point dataset. */ p->input = gal_fits_img_read_to_type(p->inputname, p->cp.hdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0, 0); if(p->input->name==NULL) gal_checkset_allocate_copy("INPUT", &p->input->name); /* NoiseChisel currently only works on 2D datasets (images). */ if(p->input->ndim!=2) error(EXIT_FAILURE, 0, "%s (hdu: %s) has %zu dimensions but NoiseChisel " "can only operate on 2D datasets (images)", p->inputname, p->cp.hdu, p->input->ndim); /* If a convolved image was given, read it in. Otherwise, read the given kernel. */ if(p->convolvedname) { /* Read the input convolved image. */ p->conv = gal_fits_img_read_to_type(p->convolvedname, p->convolvedhdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0, 0); /* Make sure the convolved image is the same size as the input. */ if( gal_data_dsize_is_different(p->input, p->conv) ) error(EXIT_FAILURE, 0, "%s (hdu %s), given to `--convolved' and " "`--convolvehdu', is not the same size as NoiseChisel's " "input: %s (hdu: %s)", p->convolvedname, p->convolvedhdu, p->inputname, p->cp.hdu); } else ui_prepare_kernel(p); /* Check for blank values to help later processing. */ gal_blank_present(p->input, 1); /* Prepare the tessellation. */ ui_prepare_tiles(p); /* Allocate space for the over-all necessary arrays. */ p->binary=gal_data_alloc(NULL, GAL_TYPE_UINT8, p->input->ndim, p->input->dsize, p->input->wcs, 0, p->cp.minmapsize, NULL, "binary", NULL); p->olabel=gal_data_alloc(NULL, GAL_TYPE_INT32, p->input->ndim, p->input->dsize, p->input->wcs, 0, p->cp.minmapsize, NULL, "labels", NULL); p->binary->flag = p->olabel->flag = p->input->flag; } /**************************************************************/ /************ High level reading function *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct noisechiselparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Let the user know that processing has started. */ if(!p->cp.quiet) { printf(PROGRAM_NAME" started on %s", ctime(&p->rawtime)); printf(" - Using %zu CPU thread%s\n", p->cp.numthreads, p->cp.numthreads==1 ? "." : "s."); printf(" - Input: %s (hdu: %s)\n", p->inputname, p->cp.hdu); if(p->convolvedname) printf(" - Convolved input: %s (hdu: %s)\n", p->convolvedname, p->convolvedhdu); else { if(p->kernelname) printf(" - %s: %s (hdu: %s)\n", p->widekernelname ? "Sharp Kernel" : "Kernel", p->kernelname, p->khdu); else printf(" - %s: FWHM=2 pixel Gaussian.\n", p->widekernelname ? "Sharp Kernel" : "Kernel"); } if(p->widekernelname) printf(" - Wide Kernel: %s (hdu: %s)\n", p->widekernelname, p->wkhdu); } } /**************************************************************/ /************ Pre-finish/abort operations *************/ /**************************************************************/ void ui_abort_after_check(struct noisechiselparams *p, char *filename, char *file2name, char *description) { char *name; if(file2name) asprintf(&name, "`%s' and `%s'", filename, file2name); else asprintf(&name, "`%s'", filename); /* Let the user know that NoiseChisel is aborting. */ fprintf(stderr, "------------------------------------------------\n" "%s aborted for a check\n" "------------------------------------------------\n" "%s (%s) has been created.\n\n" "If you want %s to continue its processing AND save any " "requested check outputs, please run it again with " "`--continueaftercheck'.\n" "------------------------------------------------\n", PROGRAM_NAME, name, description, PROGRAM_NAME); /* Clean up. */ free(name); ui_free_report(p, NULL); /* Abort. */ exit(EXIT_SUCCESS); } void ui_free_report(struct noisechiselparams *p, struct timeval *t1) { /* Free the simply allocated spaces. */ free(p->cp.hdu); free(p->maxtsize); free(p->maxltsize); free(p->cp.output); if(p->skyname) free(p->skyname); if(p->detskyname) free(p->detskyname); if(p->qthreshname) free(p->qthreshname); if(p->detsn_s_name) free(p->detsn_s_name); if(p->detsn_d_name) free(p->detsn_d_name); if(p->detectionname) free(p->detectionname); if(p->clumpsn_s_name) free(p->clumpsn_s_name); if(p->clumpsn_d_name) free(p->clumpsn_d_name); if(p->segmentationname) free(p->segmentationname); /* Free the allocated datasets. */ gal_data_free(p->sky); gal_data_free(p->std); gal_data_free(p->conv); gal_data_free(p->wconv); gal_data_free(p->input); gal_data_free(p->kernel); gal_data_free(p->binary); gal_data_free(p->olabel); gal_data_free(p->clabel); gal_data_free(p->widekernel); /* Clean up the tile structure. */ p->ltl.numchannels=NULL; gal_tile_full_free_contents(&p->ltl); gal_tile_full_free_contents(&p->cp.tl); /* Print the final message. */ if(!p->cp.quiet && t1) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/main.c�����������������������������������������������������������������0000644�0001750�0001750�00000003123�13121462410�014277� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* NoiseChisel - Detect and segment signal in a noisy dataset. NoiseChisel is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "noisechisel.h" /* Main function */ int main (int argc, char *argv[]) { struct timeval t1; struct noisechiselparams p={{{0},0},{0},0}; /* Set they starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ noisechisel(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/Makefile.in������������������������������������������������������������0000644�0001750�0001750�00000212576�13217217705�015305� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from 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= @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = 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����������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/astnoisechisel.conf����������������������������������������������������0000644�0001750�0001750�00000003215�13177434204�017110� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for NoiseChisel. # NoiseChisel is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astnoisechisel --help # Full list of options, short doc. # $ astnoisechisel -P # Print all options and used values. # $ info astnoisechisel # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Input: khdu 1 wkhdu 1 convolvedhdu 1 minskyfrac 0.7 minnumfalse 100 # Tessellation largetilesize 200,200 # Detection: mirrordist 1.5 modmedqdiff 0.01 qthresh 0.3 qthreshtilequant 1.0 smoothwidth 3 erode 2 erodengb 4 noerodequant 0.9331 opening 1 openingngb 8 sigmaclip 3,0.2 dthresh 0.0 detsnminarea 10 detquant 0.95 detgrowquant 0.70 detgrowmaxholesize 100 # Segmentation segsnminarea 15 keepmaxnearriver 0 segquant 0.95 gthresh 0.5 minriverlength 15 objbordersn 1 # Operating mode continueaftercheck 0 �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/noisechisel/Makefile.am������������������������������������������������������������0000644�0001750�0001750�00000003014�13216276304�015254� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2016, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astnoisechisel astnoisechisel_LDADD = -lgnuastro astnoisechisel_SOURCES = main.c ui.c clumps.c detection.c noisechisel.c \ sky.c segmentation.c threshold.c EXTRA_DIST = main.h authors-cite.h args.h ui.h clumps.h detection.h \ noisechisel.h segmentation.h sky.h threshold.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astnoisechisel.conf ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/����������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220467�012273� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/profiles.h������������������������������������������������������������������0000644�0001750�0001750�00000003135�13134433053�014204� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef PROFILES_H #define PROFILES_H double profiles_radial_distance(struct mkonthread *mkp); double profiles_gaussian_total(double q); double profiles_gaussian(struct mkonthread *mkp); double profiles_moffat_alpha(double fwhm, double beta); double profiles_moffat_total(double alpha, double beta, double q); double profiles_moffat(struct mkonthread *mkp); double profiles_sersic_b(double n); double profiles_sersic_total(double n, double re, double b, double q); double profiles_sersic(struct mkonthread *mkp); double profiles_circumference(struct mkonthread *mkp); double profiles_flat(struct mkonthread *mkp); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/oneprofile.h����������������������������������������������������������������0000644�0001750�0001750�00000002272�13132200542�014515� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/******************************************************************** MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ONEPROFILE_H #define ONEPROFILE_H #include "mkprof.h" int oneprofile_ispsf(uint8_t fcolvalue); void oneprof_set_prof_params(struct mkonthread *mkp); void oneprofile_make(struct mkonthread *mkp); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/mkprof.h��������������������������������������������������������������������0000644�0001750�0001750�00000006627�13216276304�013675� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MOCKGALS_H #define MOCKGALS_H #include <gnuastro/threads.h> #include "main.h" struct mkonthread { /* General parameters: */ double r; /* Elliptical radius at this point. */ double coord[2]; /* Pixel coordinate. */ double lower[2]; /* Coordinates of lower pixel position. */ double higher[2]; /* Coordinates of higher pixel position. */ double c[1]; /* Cosine of position angle(s). */ double s[1]; /* Sine of position angle(s). */ double q[1]; /* Axis ratio(s). */ double center[2]; /* Center (in FITS) in oversampled image.*/ double (*profile)(struct mkonthread *); /* Function to use. */ double truncr; /* Truncation radius in pixels. */ double intruncr; /* Inner truncation radius in pixels. */ long width[2]; /* Enclosing box in FITS axes, not C. */ float peakflux; /* Flux at profile peak. */ float brightness; /* The brightness of the profile. */ uint8_t func; /* Radial function of the profile. */ long *onaxes; /* Sides of the unover-sampled image. */ long fpixel_i[2]; /* fpixel_i before running overlap. */ int correction; /* ==1: correct the pixels afterwards. */ /* Random number generator: */ gsl_rng *rng; /* Copy of main random number generator. */ /* Profile specific parameters: */ double sersic_re; /* r/re in Sersic profile. */ double sersic_inv_n; /* Sersic index of Sersic profile. */ double sersic_nb; /* Negative of b(n) constant. */ double moffat_alphasq; /* r divided by alpha in Moffat. */ double moffat_nb; /* Negative beta in the Moffat. */ double gaussian_c; /* Constant value in Gaussian. */ double fixedvalue; /* Value of a point source. */ /* General parameters */ struct mkprofparams *p; /* Pointer to the main.h structure. */ size_t *indexs; /* Indexs to build on this thread. */ pthread_barrier_t *b; /* Pthread barrier pointer. */ struct builtqueue *ibq; /* Internally built queue. */ }; void mkprof(struct mkprofparams *p); #endif ���������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/ui.h������������������������������������������������������������������������0000644�0001750�0001750�00000004766�13216276304�013016� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_PROFILES = GAL_OPTIONS_GROUP_AFTER_COMMON, UI_GROUP_CATALOG, UI_GROUP_WCS, }; /* Keys for each option. Available letters (-V which is used by GNU is also removed): a b d g j l n u v y A G H J L O Q W Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_BACKGROUND = 'k', UI_KEY_BACKHDU = 'B', UI_KEY_NAXIS = 'x', UI_KEY_CLEARCANVAS = 'C', UI_KEY_KERNEL = 'E', UI_KEY_OVERSAMPLE = 's', UI_KEY_INDIVIDUAL = 'i', UI_KEY_NOMERGED = 'm', UI_KEY_NUMRANDOM = 'r', UI_KEY_TOLERANCE = 't', UI_KEY_TUNITINP = 'p', UI_KEY_SHIFT = 'X', UI_KEY_PREPFORCONV = 'c', UI_KEY_ZEROPOINT = 'z', UI_KEY_CIRCUMWIDTH = 'w', UI_KEY_REPLACE = 'R', UI_KEY_ENVSEED = 'e', UI_KEY_MFORFLATPIX = 'f', /* Only with long version. */ UI_KEY_PSFINIMG = 1000, UI_KEY_MAGATPEAK, UI_KEY_MCOLISBRIGHTNESS, UI_KEY_MODE, UI_KEY_CCOL, UI_KEY_FCOL, UI_KEY_RCOL, UI_KEY_NCOL, UI_KEY_PCOL, UI_KEY_QCOL, UI_KEY_MCOL, UI_KEY_TCOL, UI_KEY_CRPIX, UI_KEY_CRVAL, UI_KEY_CDELT, UI_KEY_PC, UI_KEY_CUNIT, UI_KEY_CTYPE, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct mkprofparams *p); void ui_free_report(struct mkprofparams *p, struct timeval *t1); #endif ����������gnuastro-0.5/bin/mkprof/args.h����������������������������������������������������������������������0000644�0001750�0001750�00000030256�13216276304�013326� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Option definition array. */ struct argp_option program_options[] = { { "background", UI_KEY_BACKGROUND, "STR", 0, "A background image to make the profiles on.", GAL_OPTIONS_GROUP_INPUT, &p->backname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "backhdu", UI_KEY_BACKHDU, "INT/STR", 0, "HDU of background image.", GAL_OPTIONS_GROUP_INPUT, &p->backhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "clearcanvas", UI_KEY_CLEARCANVAS, 0, 0, "All pixels in background image read as zero.", GAL_OPTIONS_GROUP_INPUT, &p->clearcanvas, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "kernel", UI_KEY_KERNEL, "STR", 0, "Parameters to only build one kernel.", GAL_OPTIONS_GROUP_INPUT, &p->kernel, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_parse_kernel }, { "naxis", UI_KEY_NAXIS, "INT[,INT,...]", 0, "Merged image size along each dimension.", GAL_OPTIONS_GROUP_OUTPUT, &p->dsize, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_sizes_reverse }, { "oversample", UI_KEY_OVERSAMPLE, "INT", 0, "Scale of oversampling (>0 and odd).", GAL_OPTIONS_GROUP_OUTPUT, &p->oversample, GAL_TYPE_UINT8, GAL_OPTIONS_RANGE_GT_0_ODD, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "psfinimg", UI_KEY_PSFINIMG, 0, 0, "PSF profiles made with all in output image.", GAL_OPTIONS_GROUP_OUTPUT, &p->psfinimg, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "individual", UI_KEY_INDIVIDUAL, 0, 0, "Build all profiles separately.", GAL_OPTIONS_GROUP_OUTPUT, &p->individual, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "nomerged", UI_KEY_NOMERGED, 0, 0, "Do not create a merged image of all profiles.", GAL_OPTIONS_GROUP_OUTPUT, &p->nomerged, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Profiles:", UI_GROUP_PROFILES }, { "mode", UI_KEY_MODE, "STR", 0, "Mode of `--ccol': `img' or `wcs'.", UI_GROUP_PROFILES, &p->mode, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET, ui_parse_coordinate_mode }, { "numrandom", UI_KEY_NUMRANDOM, "INT", 0, "No. of random points in Monte Carlo integration.", UI_GROUP_PROFILES, &p->numrandom, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "envseed", UI_KEY_ENVSEED, 0, 0, "Use GSL_RNG_SEED environment variable for seed.", UI_GROUP_PROFILES, &p->envseed, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "tolerance", UI_KEY_TOLERANCE, "FLT", 0, "Tolerance to switch to less accurate method.", UI_GROUP_PROFILES, &p->tolerance, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "tunitinp", UI_KEY_TUNITINP, 0, 0, "Truncation is in units of pixels, not radius.", UI_GROUP_PROFILES, &p->tunitinp, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "mforflatpix", UI_KEY_MFORFLATPIX, 0, 0, "mcol is flat pixel value (when fcol is 5 or 6)", UI_GROUP_PROFILES, &p->mforflatpix, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "mcolisbrightness", UI_KEY_MCOLISBRIGHTNESS, 0, 0, "mcol is total brightness, not magnitude.", UI_GROUP_PROFILES, &p->mcolisbrightness, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "shift", UI_KEY_SHIFT, "INT[, ...]", 0, "Shift profile centers in output image.", UI_GROUP_PROFILES, &p->shift, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_sizes_reverse }, { "prepforconv", UI_KEY_PREPFORCONV, 0, 0, "Shift and expand based on first catalog PSF.", UI_GROUP_PROFILES, &p->prepforconv, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "zeropoint", UI_KEY_ZEROPOINT, "FLT", 0, "Magnitude zero point.", UI_GROUP_PROFILES, &p->zeropoint, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "magatpeak", UI_KEY_MAGATPEAK, 0, 0, "Magnitude is for peak pixel, not full profile.", UI_GROUP_PROFILES, &p->magatpeak, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "circumwidth", UI_KEY_CIRCUMWIDTH, "FLT", 0, "Width of circumference (inward) profiles", UI_GROUP_PROFILES, &p->circumwidth, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "replace", UI_KEY_REPLACE, 0, 0, "Replace overlapping profile pixels, don't add.", UI_GROUP_PROFILES, &p->replace, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Columns, by info (see `--searchin'), or number (starting from 1):", UI_GROUP_CATALOG }, { "ccol", UI_KEY_CCOL, "STR/INT", 0, "Coordinate columns (one call for each dimension).", UI_GROUP_CATALOG, &p->ccol, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "fcol", UI_KEY_FCOL, "STR/INT", 0, "sersic (1), moffat (2), gaussian (3), point (4), " "flat (5), circumference (6), distance (7).", UI_GROUP_CATALOG, &p->fcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "rcol", UI_KEY_RCOL, "STR/INT", 0, "Effective radius or FWHM in pixels.", UI_GROUP_CATALOG, &p->rcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "ncol", UI_KEY_NCOL, "STR/INT", 0, "Sersic index or Moffat beta.", UI_GROUP_CATALOG, &p->ncol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "pcol", UI_KEY_PCOL, "STR/INT", 0, "Position angle.", UI_GROUP_CATALOG, &p->pcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "qcol", UI_KEY_QCOL, "STR/INT", 0, "Axis ratio.", UI_GROUP_CATALOG, &p->qcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "mcol", UI_KEY_MCOL, "STR/INT", 0, "Magnitude.", UI_GROUP_CATALOG, &p->mcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "tcol", UI_KEY_TCOL, "STR/INT", 0, "Truncation in units of --rcol, unless --tunitinp.", UI_GROUP_CATALOG, &p->tcol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "WCS parameters:", UI_GROUP_WCS }, { "crpix", UI_KEY_CRPIX, "FLT[, ...]", 0, "Pixel coordinates of reference point.", UI_GROUP_WCS, &p->crpix, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, { "crval", UI_KEY_CRVAL, "FLT[, ...]", 0, "WCS coordinates of reference point.", UI_GROUP_WCS, &p->crval, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, { "cdelt", UI_KEY_CDELT, "FLT[, ...]", 0, "Resolution in each dimension.", UI_GROUP_WCS, &p->cdelt, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, { "pc", UI_KEY_PC, "FLT[, ...]", 0, "WCS rotation matrix (all elements).", UI_GROUP_WCS, &p->pc, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, { "cunit", UI_KEY_CUNIT, "STR[, ... ]", 0, "Units of the WCS coordinates (e.g., `deg').", UI_GROUP_WCS, &p->cunit, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_strings }, { "ctype", UI_KEY_CTYPE, "STR[, ... ]", 0, "One of FITS standard WCS types.", UI_GROUP_WCS, &p->ctype, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_strings }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/authors-cite.h��������������������������������������������������������������0000644�0001750�0001750�00000002773�13211076737�015007� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif �����gnuastro-0.5/bin/mkprof/main.h����������������������������������������������������������������������0000644�0001750�0001750�00000021152�13216276304�013311� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include <pthread.h> #include <gsl/gsl_rng.h> #include <gnuastro/fits.h> #include <gnuastro-internal/options.h> /* Progarm name macros: */ #define PROGRAM_NAME "MakeProfiles" /* Program full name. */ #define PROGRAM_EXEC "astmkprof" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Some constants */ #define EPSREL_FOR_INTEG 2 #define DEGREESTORADIANS M_PI/180.0 /* Modes to interpret coordinates. */ enum coord_modes { MKPROF_MODE_INVALID, /* For sanity checks. */ MKPROF_MODE_IMG, /* Use image coordinates. */ MKPROF_MODE_WCS, /* Use WCS coordinates. */ }; /* Types of profiles. */ enum profile_types { PROFILE_INVALID, /* Invalid (=0 by C standard). */ PROFILE_SERSIC, /* Sersic profile. */ PROFILE_MOFFAT, /* Moffat Profile. */ PROFILE_GAUSSIAN, /* Gaussian Profile. */ PROFILE_POINT, /* Point profile. */ PROFILE_FLAT, /* Flat profile. */ PROFILE_CIRCUMFERENCE, /* Circumference profile. */ PROFILE_DISTANCE, /* Elliptical radius of pixel. */ PROFILE_MAXIMUM_CODE, /* Just for a sanity check. */ }; #define MINCIRCUMWIDTH 0.5f /* Log file: 0: ID. 1: Overlap magnitude. 2: Number of accurate pixels. 3: Fraction of accurate values. 4: Is individual file created? */ #define LOGNUMCOLS 5 #define LOGFILENAME PROGRAM_EXEC".log" struct builtqueue { size_t id; /* ID of this object. */ int ispsf; /* This is a PSF profile. */ int overlaps; /* ==1: Overlaps with the image. */ gal_data_t *image; /* Array of this profile's image. */ gal_data_t *overlap_i; /* Overlap tile over individual array. */ gal_data_t *overlap_m; /* Overlap tile over merged array. */ int func; /* Profile's radial function. */ int indivcreated; /* ==1: an individual file is created. */ size_t numaccu; /* Number of accurate pixels. */ double accufrac; /* Difference of accurate values. */ struct builtqueue *next; /* Pointer to next element. */ }; struct mkprofparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ char *backname; /* Name of background image file name. */ char *catname; /* Name of catalog of parameters. */ char *backhdu; /* HDU of background image. */ size_t *dsize; /* Size of the output image. */ uint8_t clearcanvas; /* Pixels in background image set to zero. */ gal_data_t *kernel; /* Parameters to define a kernel. */ uint8_t oversample; /* Oversampling scale. */ uint8_t psfinimg; /* ==1: Build PSF profiles in image. */ uint8_t individual; /* ==1: Build all catalog separately. */ uint8_t nomerged; /* ==1: Don't make a merged image of all. */ char *typestr; /* Type of finally merged output image. */ size_t numrandom; /* Number of radom points for integration. */ float tolerance; /* Accuracy to stop integration. */ uint8_t tunitinp; /* ==1: Truncation is in pixels, not radial.*/ size_t *shift; /* Shift along axeses position of profiles. */ uint8_t prepforconv; /* Shift and expand by size of first psf. */ float zeropoint; /* Magnitude of zero point flux. */ double circumwidth; /* Width of circumference (inward). */ uint8_t replace; /* Replace overlaping profile pixel values. */ uint8_t magatpeak; /* Mag only for peak pixel, not all profile.*/ uint8_t envseed; /* Use GSL_RNG_SEED for random seed. */ uint8_t mode; /* Coordinates in WCS or image standard. */ gal_list_str_t *ccol; /* Columns that keep coordinates. */ char *fcol; /* Column specifying profile function. */ char *rcol; /* Effective radius of profile. */ char *ncol; /* Sersic index column of profile. */ char *pcol; /* Position angle column of profile. */ char *qcol; /* Axis ratio column of profile. */ char *mcol; /* Magnitude column. */ char *tcol; /* Truncation of the profiles. */ uint8_t mforflatpix; /* mcol is flat pixel value (f is 4 or 5). */ uint8_t mcolisbrightness; /* mcol is total brightness not magnitude. */ gal_data_t *crpix; /* CRPIX FITS header keywords. */ gal_data_t *crval; /* CRVAL FITS header keywords. */ gal_data_t *cdelt; /* For CDELTi FITS header keywords. */ gal_data_t *pc; /* WCS PC matrix. */ gal_data_t *cunit; /* Units of each coordinate. */ gal_data_t *ctype; /* Type of the coordinates. */ /* Output */ gal_data_t *out; /* Output image. */ char *outdir; /* Output directory. */ char *basename; /* Merged image name with no directory. */ /* Processing parameters: */ size_t num; /* The number of profiles. */ double *x; /* X axis position of profile center. */ double *y; /* Y axis position of profile center. */ uint8_t *f; /* Profile function code. */ float *r; /* Radius of profile. */ float *n; /* Index of profile. */ float *p; /* Position angle of profile. */ float *q; /* Axis ratio of profile. */ float *m; /* Magnitude of profile. */ float *t; /* Truncation distance. */ gsl_rng *rng; /* Main instance of random number generator.*/ time_t rawtime; /* Starting time of the program. */ double *cat; /* Input catalog. */ gal_data_t *log; /* Log data to be printed. */ struct builtqueue *bq; /* Top (last) elem of build queue. */ pthread_cond_t qready; /* bq is ready to be written. */ pthread_mutex_t qlock; /* Mutex lock to change builtq. */ double halfpixel; /* Half pixel in oversampled image. */ char *wcsheader; /* The WCS header information for main img. */ int wcsnkeyrec; /* The number of keywords in the WCS header.*/ char *mergedimgname; /* Name of merged image. */ int nwcs; /* for WCSLIB: no. coord. representations. */ struct wcsprm *wcs; /* WCS information for this dataset. */ size_t ndim; /* Number of dimensions (for `nomerged'). */ /* We can't put it in `out' because it is */ /* meaning ful there. */ }; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/profiles.c������������������������������������������������������������������0000644�0001750�0001750�00000010121�13134502440�014165� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <stdlib.h> #include <gsl/gsl_sf_gamma.h> /* For total Sersic brightness. */ #include "main.h" #include "mkprof.h" /* Needs main.h, astrthreads.h */ #include "profiles.h" /**************************************************************** ***************** Profiles: ******************** ****************************************************************/ /* The Gaussian function at a point. */ double profiles_radial_distance(struct mkonthread *mkp) { return mkp->r; } /* The integral of the Gaussian from -inf to +inf equals the square root of PI. So from zero to +inf it equals half of that.*/ double profiles_gaussian_total(double q) { return q*sqrt(M_PI)/2; } /* The Gaussian function at a point. */ double profiles_gaussian(struct mkonthread *mkp) { return exp( mkp->gaussian_c * mkp->r * mkp->r ); } /* This function will find the moffat function alpha value based on the explantions here: http://labs.adsabs.harvard.edu/adsabs/abs/2001MNRAS.328..977T/ alpha=(FWHM/2)/(2^(1.0/beta)-1)^(0.5). Then the moffat function at r is: (1.0 + (r/alpha)^2.0)^(-1.0*beta)*/ double profiles_moffat_alpha(double fwhm, double beta) { return (fwhm/2)/pow((pow(2, 1/beta)-1), 0.5f); } /* Find the total value of the Moffat profile. I am using equation 10 from Pengetal 2010 (Galfit). In finding the profiles, I am assuming \Sigma_0=1. So that is what I put here too.*/ double profiles_moffat_total(double alpha, double beta, double q) { return M_PI*alpha*alpha*q/(beta-1); } /* Find the Moffat profile for a certain radius. rda=r/alpha and nb=-1*b. This is done before hand to speed up the process. */ double profiles_moffat(struct mkonthread *mkp) { return pow(1+mkp->r*mkp->r/mkp->moffat_alphasq, mkp->moffat_nb); } /* This approximation of b(n) for n>0.35 is taken from McArthur, Courteau and Holtzman 2003: http://adsabs.harvard.edu/abs/2003ApJ...582..689 */ double profiles_sersic_b(double n) { if(n<=0.35f) error(EXIT_FAILURE, 0, "the Sersic index cannot be smaller " "than 0.35. It is %.3f", n); return 2*n-(1/3)+(4/(405*n))+(46/(25515*n*n))+ (131/(1148175*n*n*n)-(2194697/(30690717750*n*n*n*n))); } /* Find the total brightness in a Sersic profile. From equation 4 in Peng 2010. This assumes the surface brightness at the effective radius is 1.*/ double profiles_sersic_total(double n, double re, double b, double q) { return (2*M_PI*re*re*exp(b)*n*pow(b, -2*n)*q* gsl_sf_gamma(2*n)); } /* Find the Sersic profile for a certain radius. rdre=r/re, inv_n=1/n, nb= -1*b. */ double profiles_sersic(struct mkonthread *mkp) { return exp( mkp->sersic_nb * ( pow(mkp->r/mkp->sersic_re, mkp->sersic_inv_n) -1 ) ); } /* Make a circumference (inner to the radius). */ double profiles_circumference(struct mkonthread *mkp) { return mkp->r > mkp->intruncr ? mkp->fixedvalue : 0.0f; } /* Always returns a fixed value: */ double profiles_flat(struct mkonthread *mkp) { return mkp->fixedvalue; } �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/oneprofile.c����������������������������������������������������������������0000644�0001750�0001750�00000045250�13216276304�014527� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/******************************************************************** MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <sys/time.h> /* generate random seed */ #include <gsl/gsl_rng.h> /* used in setrandoms */ #include <gsl/gsl_randist.h> /* To make noise. */ #include <gsl/gsl_integration.h> /* gsl_integration_qng */ #include <gnuastro/fits.h> #include <gnuastro/dimension.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "mkprof.h" /* Needs main.h and astrthreads.h */ #include "profiles.h" #include "oneprofile.h" /**************************************************************** ************** Radial distance ****************** ****************************************************************/ /* Set the center position of the profile in the oversampled image. Note that `mkp->width' is in the non-oversampled scale. IMPORTANT: the ordering is in FITS coordinate order. */ static void oneprofile_center_oversampled(struct mkonthread *mkp) { struct mkprofparams *p=mkp->p; double *dim; long os=p->oversample; size_t i, id=mkp->ibq->id; double val, pixfrac, intpart; for(i=0;i<p->ndim;++i) { dim = i==0 ? p->x : p->y; pixfrac = modf(fabs(dim[id]), &intpart); val = ( os*(mkp->width[i]/2 + pixfrac) + (pixfrac<0.5f ? os/2 : -1*os/2-1) ); mkp->center[i] = round(val*100)/100; } } static void oneprofile_set_coord(struct mkonthread *mkp, size_t index) { size_t i, coord_c[2]; uint8_t os=mkp->p->oversample; size_t ndim=mkp->ibq->image->ndim, *dsize=mkp->ibq->image->dsize; /* Get the coordinates in C order. */ gal_dimension_index_to_coord(index, ndim, dsize, coord_c); /* Convert these coordinates to one where the profile center is at the center and the image is not over-sampled. Note that only `coord_c' is in C order.*/ for(i=0;i<ndim;++i) mkp->coord[i] = ( coord_c[ndim-i-1] - mkp->center[i] )/os; } /* Convert cartesian coordinates to the rotated elliptical radius. See the "Defining an ellipse" section of the book for the full derivation. */ static void oneprofile_r_el(struct mkonthread *mkp) { double Xr, Yr; /* Rotated x and y. */ double q=mkp->q[0]; double c=mkp->c[0], s=mkp->s[0]; double x=mkp->coord[0], y=mkp->coord[1]; Xr = x * ( c ) + y * ( s ); Yr = x * ( -1.0f*s ) + y * ( c ); mkp->r = sqrt( Xr*Xr + Yr*Yr/q/q ); } /* Calculate the circular/spherical distance of a pixel to the profile center. This is just used to add pixels in the stack. Later, when the pixels are popped from the stack, the elliptical radius will be used to give them a value.*/ static float oneprofile_r_circle(size_t index, struct mkonthread *mkp) { size_t i, c[2]; double d, sum=0.0f; size_t ndim=mkp->ibq->image->ndim, *dsize=mkp->ibq->image->dsize; /* Convert the index into a coordinate. */ gal_dimension_index_to_coord(index, ndim, dsize, c); /* Find the distance to the center along each dimension (in FITS order). */ for(i=0;i<ndim;++i) { d = c[ndim-i-1] - mkp->center[i]; sum += d*d; } /* Return the distance. */ return sqrt(sum); } /**************************************************************** ************** Random points ****************** ****************************************************************/ /* Fill pixel with random values */ float oneprofile_randompoints(struct mkonthread *mkp) { double range[2], sum=0.0f; size_t i, j, numrandom=mkp->p->numrandom, ndim=mkp->p->ndim; /* Set the range in each dimension. */ for(i=0;i<ndim;++i) range[i] = mkp->higher[i] - mkp->lower[i]; /* Find the sum of the profile on the random positions. */ for(i=0;i<numrandom;++i) { for(j=0;j<ndim;++j) mkp->coord[j] = mkp->lower[j] + gsl_rng_uniform(mkp->rng) * range[j]; oneprofile_r_el(mkp); sum+=mkp->profile(mkp); } return sum/numrandom; } /**************************************************************** ***************** 2D integration ******************** ****************************************************************/ /* This is an old implementation which we are not using now. But it is kept here in case it can be useful */ #if 0 double twod_over_x(double x, void *params) { struct mkonthread *mkp=(struct mkonthread *) params; mkp->x=x; oneprofile_r_el(mkp); return mkp->profile(mkp); } /* Find the 2d integration over the region. */ double twod_over_xy(double y, void *params) { gsl_function F; static double abserr; static size_t neval=0; double epsabs=0, epsrel=EPSREL_FOR_INTEG, result; struct mkonthread *mkp=(struct mkonthread *) params; F.function = &twod_over_x; F.params = params; mkp->y=y; gsl_integration_qng(&F, mkp->xl, mkp->xh, epsabs, epsrel, &result, &abserr, &neval); return result; } /* 2D integration of a profile.*/ double integ2d(struct mkonthread *mkp) { gsl_function F; static double abserr; static size_t neval=0; double epsabs=0, epsrel=EPSREL_FOR_INTEG, result; F.function = &twod_over_xy; F.params = mkp; gsl_integration_qng(&F, mkp->yl, mkp->yh, epsabs, epsrel, &result, &abserr, &neval); return result; } #endif /**************************************************************/ /************ Pixel by pixel building *************/ /********* Positions are in C not FITS *********/ /**************************************************************/ /* `oneprofile_center_oversampled' stored the center of the profile in floating point coordinates. This function will convert that into a pixel index. */ static size_t oneprofile_center_pix_index(struct mkonthread *mkp) { double pixfrac, intpart; size_t *dsize=mkp->ibq->image->dsize; size_t i, coord[2], ndim=mkp->p->ndim; /* Find the coordinates of the center point. Note `mkp->center' is in FITS coordinates, while coord must be in C coordinates (to be used in `gal_dimension_coord_to_index'). */ for(i=0;i<ndim;++i) { pixfrac = modf(mkp->center[i], &intpart); coord[ndim-i-1] = (long)(mkp->center[i]) + ( pixfrac<0.5f ? 0 : 1 ); } /* Retun the pixel index of this coordinate. */ return gal_dimension_coord_to_index(ndim, dsize, coord); } static void oneprofile_pix_by_pix(struct mkonthread *mkp) { struct builtqueue *ibq=mkp->ibq; size_t ndim=ibq->image->ndim, *dsize=ibq->image->dsize; uint8_t *byt; gal_list_sizet_t *Q=NULL; int use_rand_points=1, ispeak=1; double tolerance=mkp->p->tolerance; float circ_r, *array=mkp->ibq->image->array; double (*profile)(struct mkonthread *)=mkp->profile; double truncr=mkp->truncr, approx, hp=0.5f/mkp->p->oversample; size_t i, p, *dinc=gal_dimension_increment(ndim, dsize); /* lQ: Largest. sQ: Smallest in queue */ gal_list_dosizet_t *lQ=NULL, *sQ; /* Find the nearest pixel to the profile center and add it to the queue. */ p=oneprofile_center_pix_index(mkp); /* If this is a point source, just fill that one pixel and leave this function. */ if(mkp->func==PROFILE_POINT) { array[p]=1; return; } /* Allocate the `byt' array. It is used as a flag to make sure that we don't re-calculate the profile value on a pixel more than once. */ byt = gal_data_calloc_array(GAL_TYPE_UINT8, gal_dimension_total_size(ndim, dsize), __func__, "byt"); /* Start the queue: */ byt[p]=1; gal_list_dosizet_add( &lQ, &sQ, p, oneprofile_r_circle(p, mkp) ); /* If random points are necessary, then do it: */ switch(mkp->func) { case PROFILE_SERSIC: case PROFILE_MOFFAT: case PROFILE_GAUSSIAN: while(sQ) { /* In case you want to see the status of the twosided ordered queue, increasing and decreasing side by side, uncomment this line. Note that there will be a lot of lines printed! */ /*print_tossll(lQ, sQ);*/ /* Pop a pixel from the queue, convert its index into coordinates and use them to estimate the elliptical radius of the pixel. If the pixel is outside the truncation radius, ignore it. */ p=gal_list_dosizet_pop_smallest(&lQ, &sQ, &circ_r); oneprofile_set_coord(mkp, p); oneprofile_r_el(mkp); if(mkp->r > truncr) continue; /* Find the value for this pixel: */ for(i=0;i<ndim;++i) { mkp->lower[i] = mkp->coord[i] - hp; mkp->higher[i] = mkp->coord[i] + hp; } /* Find the random points and profile center. */ array[p]=oneprofile_randompoints(mkp); approx=profile(mkp); if (fabs(array[p]-approx)/array[p] < tolerance) use_rand_points=0; /* Save the peak flux if this is the first pixel: */ if(ispeak) { mkp->peakflux=array[p]; ispeak=0; } /* For the log file: */ ++ibq->numaccu; ibq->accufrac+=array[p]; /* Go over the neighbors and add them to queue of elements to check if they haven't been done already. */ GAL_DIMENSION_NEIGHBOR_OP(p, ndim, dsize, 1, dinc, { if(byt[nind]==0) { byt[nind]=1; gal_list_dosizet_add( &lQ, &sQ, nind, oneprofile_r_circle(nind, mkp) ); } } ); if(use_rand_points==0) break; } } /* All the pixels that required integration or random points are now done, so we don't need an ordered array any more. */ gal_list_dosizet_to_sizet(lQ, &Q); /* Order doesn't matter any more, add all the pixels you find. */ while(Q) { p=gal_list_sizet_pop(&Q); oneprofile_set_coord(mkp, p); oneprofile_r_el(mkp); /* See if this pixel's radial distance is larger than the truncation radius. If so, then don't add its neighbors to the queue and continue to the next pixel in the queue. */ if(mkp->r>truncr) { /* For the circumference, if the profile is too elongated and circumwidth is too small, then some parts of the circumference will not be shown without this condition. */ if(mkp->func==PROFILE_CIRCUMFERENCE) array[p]=profile(mkp); continue; } /* Find the value for this pixel: */ array[p]=profile(mkp); /* Save the peak flux if this is the first pixel: */ if(ispeak) { mkp->peakflux=array[p]; ispeak=0; } /* Go over the neighbours and add them to queue of elements to check. */ GAL_DIMENSION_NEIGHBOR_OP(p, ndim, dsize, 1, dinc, { if(byt[nind]==0) { byt[nind]=1; gal_list_sizet_add(&Q, nind); } } ); } /* Clean up. */ free(byt); free(dinc); } /**************************************************************/ /************ Set profile parameters *************/ /**************************************************************/ int oneprofile_ispsf(uint8_t fcode) { return fcode==PROFILE_MOFFAT || fcode==PROFILE_GAUSSIAN; } /* Prepare all the parameters for any type of profile. */ void oneprof_set_prof_params(struct mkonthread *mkp) { struct mkprofparams *p=mkp->p; double sigma; int tp=p->tunitinp; size_t id=mkp->ibq->id; /* Fill the most basic profile agnostic parameters. */ mkp->brightness = ( p->mcolisbrightness ? p->m[id] : pow( 10, (p->zeropoint - p->m[id]) / 2.5f ) ); mkp->ibq->ispsf = p->kernel ? 1 : oneprofile_ispsf(p->f[id]); mkp->func = mkp->ibq->func = p->f[id]; /* Shifts were already multiplied with oversample. Just note that p->x and p->y are in the FITS ordering, while p->shift is in C ordering. */ mkp->q[0] = p->q[id]; p->x[id] += p->shift[1]/p->oversample; p->y[id] += p->shift[0]/p->oversample; mkp->c[0] = cos( p->p[id] * DEGREESTORADIANS ); mkp->s[0] = sin( p->p[id] * DEGREESTORADIANS ); /* Fill the profile-dependent parameters. */ switch (mkp->func) { case PROFILE_SERSIC: mkp->correction = 1; mkp->profile = &profiles_sersic; mkp->sersic_re = p->r[id]; mkp->sersic_inv_n = 1.0f/p->n[id]; mkp->sersic_nb = -1.0f*profiles_sersic_b(p->n[id]); mkp->truncr = tp ? p->t[id] : p->t[id]*p->r[id]; break; case PROFILE_MOFFAT: mkp->correction = 1; mkp->profile = &profiles_moffat; mkp->moffat_nb = -1.0f*p->n[id]; mkp->moffat_alphasq = profiles_moffat_alpha(p->r[id], p->n[id]); mkp->moffat_alphasq *= mkp->moffat_alphasq; mkp->truncr = tp ? p->t[id] : p->t[id]*p->r[id]/2; if(p->psfinimg==0 && p->individual==0) { mkp->brightness = 1.0f; /* When the PSF is a separate image, */ p->x[id] = 0.0f; /* it should be centered and have a */ p->y[id] = 0.0f; /* total brightness of 1.0f. */ } break; case PROFILE_GAUSSIAN: mkp->correction = 1; mkp->profile = &profiles_gaussian; sigma = p->r[id]/2.35482f; mkp->gaussian_c = -1.0f/(2.0f*sigma*sigma); mkp->truncr = tp ? p->t[id] : p->t[id]*p->r[id]/2; if(p->psfinimg==0 && p->individual==0) { mkp->brightness = 1.0f; /* Same as the explanations for */ p->x[id] = 0.0f; /* The Moffat profile. */ p->y[id] = 0.0f; } break; case PROFILE_POINT: mkp->correction = 1; mkp->fixedvalue = 1.0f; mkp->profile = &profiles_flat; break; case PROFILE_FLAT: mkp->profile = &profiles_flat; mkp->truncr = tp ? p->t[id] : p->t[id]*p->r[id]; if(p->mforflatpix) { mkp->correction = 0; mkp->fixedvalue = p->m[id]; } else { mkp->correction = 1; mkp->fixedvalue = 1.0f; } break; case PROFILE_CIRCUMFERENCE: mkp->profile = &profiles_circumference; mkp->truncr = tp ? p->t[id] : p->t[id]*p->r[id]; mkp->intruncr = mkp->truncr - p->circumwidth; if(p->mforflatpix) { mkp->correction = 0; mkp->fixedvalue = p->m[id]; } else { mkp->correction = 1; mkp->fixedvalue = 1.0f; } if(mkp->intruncr<0.0f) mkp->intruncr = 0.0f; break; case PROFILE_DISTANCE: mkp->profile = profiles_radial_distance; mkp->truncr = tp ? p->t[id] : p->t[id]*p->r[id]; mkp->correction = 0; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us so we can correct " "this problem. The profile code %u is not recognized.", __func__, mkp->func); } } /**************************************************************/ /************ Outside functions *************/ /**************************************************************/ void oneprofile_make(struct mkonthread *mkp) { struct mkprofparams *p=mkp->p; double sum; float *f, *ff; size_t i, dsize[3], ndim=p->ndim; /* Find the profile center in the over-sampled image in C coordinates. IMPORTANT: width must not be oversampled.*/ oneprofile_center_oversampled(mkp); /* From this point on, the widths will be in the actual pixel widths (with oversampling). */ for(i=0;i<ndim;++i) { mkp->width[i] *= p->oversample; dsize[ndim-i-1] = mkp->width[i]; } /* Allocate and clear the array for this one profile. */ mkp->ibq->image=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, ndim, dsize, NULL, 1, p->cp.minmapsize, "MOCK", "Brightness", NULL); /* Build the profile in the image. */ oneprofile_pix_by_pix(mkp); /* Correct the sum of pixels in the profile so it has the fixed total magnitude or pixel value, mkp->correction was set in setprofparams. Note that the profiles were not normalized during the building.*/ if(mkp->correction) { /* First get the sum of all the pixels in the profile. */ ff=(f=mkp->ibq->image->array) + mkp->ibq->image->size; sum=0.0f; do sum+=*f++; while(f<ff); /* Correct the fraction of brightness that was calculated accurately (not using the pixel center). */ mkp->ibq->accufrac /= sum; /* Correct all the profile pixels. Note that ideally, if a user wants a NaN valued profile, they should use the `flat' profile with `--mforflatpix', which won't need this correction. However, it might happen that they forget the later, or the catalog might be generated by a script that gives a NaN value for the magnitude with any kind of profile. In such cases if we don't check the NaN value, then the whole profile's box is going to be NaN values, which is inconvenient and with the simple check here we can avoid it (only have the profile's pixels set to NaN. */ ff = (f=mkp->ibq->image->array) + mkp->ibq->image->size; if(isnan(mkp->brightness)) do *f = *f ? NAN : *f ; while(++f<ff); else { if(p->magatpeak) do *f++ *= mkp->brightness/mkp->peakflux; while(f<ff); else do *f++ *= mkp->brightness/sum; while(f<ff); } } } ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/mkprof.c��������������������������������������������������������������������0000644�0001750�0001750�00000050624�13216276304�013664� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/******************************************************************** MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <float.h> #include <string.h> #include <stdlib.h> #include <gnuastro/box.h> #include <gnuastro/git.h> #include <gnuastro/fits.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "mkprof.h" /* Needs main.h astrthreads.h */ #include "oneprofile.h" /**************************************************************/ /************ builtqueue linked list *************/ /**************************************************************/ /* Add an empty element to the existing builtqueue. */ void builtqueue_addempty(struct builtqueue **bq) { struct builtqueue *tbq; /* Allocate the element. */ errno=0; tbq=malloc(sizeof *tbq); if(tbq==NULL) error(EXIT_FAILURE, 0, "%s: allocating %zu bytes for `tbq'", __func__, sizeof *tbq); /* Initialize the values (same order as in structure definition). */ tbq->id = GAL_BLANK_SIZE_T; tbq->ispsf = 0; tbq->overlaps = 0; tbq->image = NULL; tbq->overlap_i = NULL; tbq->overlap_m = NULL; tbq->func = PROFILE_MAXIMUM_CODE; tbq->indivcreated = 0; tbq->numaccu = 0; tbq->accufrac = 0.0f; /* Set its next element to the input bq and re-set the input bq. */ tbq->next=*bq; *bq=tbq; } /**************************************************************/ /************ Save individual *************/ /**************************************************************/ #define NUMBERNAMESTRLEN 100 void saveindividual(struct mkonthread *mkp) { struct mkprofparams *p=mkp->p; double *crpix; long os=p->oversample; size_t i, ndim=p->ndim; struct builtqueue *ibq=mkp->ibq; char *filename, *jobname, *outdir=p->outdir; /* Write the name and remove a similarly named file when the `--kernel' option wasn't called. If `--kernel' is called, then we should just use the final merged filename. */ if(p->kernel) filename=p->mergedimgname; else { asprintf(&filename, "%s%zu_%s", outdir, ibq->id, p->basename); gal_checkset_writable_remove(filename, 0, p->cp.dontdelete); } /* Write the array to file (a separately built PSF doesn't need WCS coordinates). */ if(ibq->ispsf && p->psfinimg==0) gal_fits_img_write(ibq->image, filename, NULL, PROGRAM_NAME); else { /* Allocate space for the corrected crpix and fill it in. Both `crpix' and `fpixel_i' are in FITS order. */ crpix=gal_data_malloc_array(GAL_TYPE_FLOAT64, ndim, __func__, "crpix"); for(i=0;i<ndim;++i) crpix[i] = ((double *)(p->crpix->array))[i] - os*(mkp->fpixel_i[i]-1); /* Write the image. */ gal_fits_img_write_corr_wcs_str(ibq->image, filename, p->wcsheader, p->wcsnkeyrec, crpix, NULL, PROGRAM_NAME); } ibq->indivcreated=1; /* Report if in verbose mode. */ if(!p->cp.quiet) { asprintf(&jobname, "%s created.", filename); gal_timing_report(NULL, jobname, 2); free(jobname); } /* Clean up. */ if(p->kernel==NULL) free(filename); } /**************************************************************/ /************ The builders *************/ /**************************************************************/ /* High-level function to built a single profile and prepare it for the next steps. */ static void mkprof_build_single(struct mkonthread *mkp, long *fpixel_i, long *lpixel_i, long *fpixel_o) { struct mkprofparams *p = mkp->p; struct builtqueue *ibq = mkp->ibq; void *ptr; int needs_crop=0; size_t i, ind, fits_i, ndim=p->ndim; size_t start_indiv[2], start_mrg[2], dsize[2], os=p->oversample; /* Make a copy of the main random number generator to use for this profile (in this thread). */ gsl_rng_memcpy(mkp->rng, p->rng); /* Set the seed of the random number generator if the environment is not to be used. */ if(mkp->p->envseed==0) gsl_rng_set(mkp->rng, gal_timing_time_based_rng_seed()); /* Make the profile */ oneprofile_make(mkp); /* Build an individual image if necessary. */ if( p->individual || (ibq->ispsf && p->psfinimg==0)) { saveindividual(mkp); if(ibq->ispsf && p->psfinimg==0) ibq->overlaps=0; } /* If we want a merged image, then a tile needs to be defined over the individual profile array and the output merged array to define the overlapping region. */ if(p->out) { /* Note that `fpixel_o' and `lpixel_o' were in the un-oversampled image, they are also in the FITS coordinates. */ for(i=0;i<ndim;++i) { /* Set the start and width of the overlap. */ fits_i = ndim-i-1; start_indiv[i] = os * (fpixel_o[fits_i] - 1); start_mrg[i] = os * (fpixel_i[fits_i] - 1); dsize[i] = os * (lpixel_i[fits_i] - fpixel_i[fits_i] + 1); /* Check if we need to crop the individual image or not. */ if(dsize[i] != ibq->image->dsize[i]) needs_crop=1; } /* Define the individual overlap tile. */ if(needs_crop) { /* If a crop is needed, set the starting pointer. */ ind=gal_dimension_coord_to_index(ndim, ibq->image->dsize, start_indiv); ptr=gal_data_ptr_increment(ibq->image->array, ind, ibq->image->type); } else ptr=ibq->image->array; ibq->overlap_i=gal_data_alloc(ptr, ibq->image->type, ndim, dsize, NULL, 0, -1, NULL, NULL, NULL); ibq->overlap_i->block=ibq->image; /* Define the merged overlap tile. */ ind=gal_dimension_coord_to_index(ndim, p->out->dsize, start_mrg); ptr=gal_data_ptr_increment(p->out->array, ind, p->out->type); ibq->overlap_m=gal_data_alloc(ptr, p->out->type, ndim, dsize, NULL, 0, -1, NULL, NULL, NULL); ibq->overlap_m->block=p->out; } } /* The profile has been built, now add it to the queue of profiles that must be written into the final merged image. */ static void mkprof_add_built_to_write_queue(struct mkonthread *mkp, struct builtqueue *ibq, struct builtqueue **fbq, size_t counter) { struct mkprofparams *p = mkp->p; int lockresult; pthread_mutex_t *qlock=&p->qlock; pthread_cond_t *qready=&p->qready; /* Try locking the mutex so no thread can change the value of p->bq. If you can lock it, then put the internal builtqueue on top of the general builtqueue. If you can't, continue adding to the internal builtqueue (make the next profiles) until you find a chance to lock the mutex. */ lockresult=pthread_mutex_trylock(qlock); if(lockresult==0) /* Mutex was successfully locked. */ { /* Add this internal queue to system queue. */ (*fbq)->next=p->bq; p->bq=ibq; /* If the list was empty when you locked the mutex, then either `mkprof_write` is waiting behind a condition variable for you to fill it up or not (either it hasn't got to setting the condition variable yet (this function locked the mutex before `mkprof_write`) or it just got the list to be made and is busy writing the arrays in the output). In either case, pthread_cond_signal will work. */ if((*fbq)->next==NULL) pthread_cond_signal(qready); pthread_mutex_unlock(qlock); /* Finally set both the internal queue and the first internal queue element to NULL.*/ (*fbq)=NULL; mkp->ibq=NULL; } /* The mutex couldn't be locked and there are no more objects for this thread to build (giving a chance for this thread to add up its built profiles). So we have to lock the mutex to pass on this built structure to the builtqueue. */ else if (mkp->indexs[counter+1]==GAL_BLANK_SIZE_T) { pthread_mutex_lock(qlock); (*fbq)->next=p->bq; p->bq=ibq; pthread_cond_signal(qready); pthread_mutex_unlock(qlock); } } /* Build the profiles that are indexed in the indexs array of the mkonthread structure that was assigned to it. See the explanation above overlap (/lib/box.c) for a complete explanation of fpixel_i, lpixel_i, fpixel_o and lpixel_o. ========================================================= About the Central x and y of each profile: The user has asked for the profile to be built on the coordinates (real numbers) of `x` and `y` in an output image in the FITS format. We are building the full image for each galaxy separately in an array with an odd number of sides which maybe oversampled. In the FITS format, the pixel centers have an integer value. So for example in 1D, a pixel whose center value is 10.00 covers the area of: [9.5,10.5). We want the fractional part of `x` (don't forget, this example is 1D) to be in the central pixel of this separate array (with odd sides) that we will be building. The result of this convention is that in 1D, a continuous space pixel with a fractional value of 0.1 is going to be after the central pixel's center, while one with a fractional value of 0.9 will be before it. In this manner, later on, when we want to find the overlap between this array and the output array, if we have a fractional value >=0.5, we will just shift the integer part of the central pixel by one and completely ignore the fractional part. */ static void * mkprof_build(void *inparam) { struct mkonthread *mkp=(struct mkonthread *)inparam; struct mkprofparams *p=mkp->p; double center[2]; size_t i, id, ndim=p->ndim; struct builtqueue *ibq, *fbq=NULL; long fpixel_i[2], lpixel_i[2], fpixel_o[2], lpixel_o[2]; /* Make each profile that was specified for this thread. */ for(i=0; mkp->indexs[i]!=GAL_BLANK_SIZE_T; ++i) { /* Create a new builtqueue element with all the information. fbq will be used when we want to add ibq to p->bq. It is defined so we don't have to waste time traversing the ibq. Its characteristic compared to the other elements of ibq is that fbq->next==NULL. So to add ibq to p->bq, we just have to set fbq->next=p->bq and then set p->bq to ibq.*/ builtqueue_addempty(&mkp->ibq); ibq=mkp->ibq; id=ibq->id=mkp->indexs[i]; if(fbq==NULL) fbq=ibq; /* Write the necessary parameters for this profile into mkp.*/ oneprof_set_prof_params(mkp); /* Find the bounding box size (NOT oversampled). */ if( p->f[id] == PROFILE_POINT ) mkp->width[0]=mkp->width[1]=1; else gal_box_bound_ellipse(mkp->truncr, mkp->q[0]*mkp->truncr, p->p[id], mkp->width); /* Get the overlapping pixels using the starting points (NOT oversampled). */ if(p->out) { center[0]=p->x[id]; center[1]=p->y[id]; gal_box_border_from_center(center, ndim, mkp->width, fpixel_i, lpixel_i); memcpy(mkp->fpixel_i, fpixel_i, ndim*sizeof *fpixel_i); ibq->overlaps = gal_box_overlap(mkp->onaxes, fpixel_i, lpixel_i, fpixel_o, lpixel_o, ndim); } /* Build the profile if necessary. */ if(ibq->overlaps || p->individual || (ibq->ispsf && p->psfinimg==0)) mkprof_build_single(mkp, fpixel_i, lpixel_i, fpixel_o); /* Add this profile to the list of profiles that must be written onto the final merged image with another thread. */ if(p->cp.numthreads>1) mkprof_add_built_to_write_queue(mkp, ibq, &fbq, i); } /* Free the allocated space for this thread and wait until all other threads finish. */ gsl_rng_free(mkp->rng); if(p->cp.numthreads==1) p->bq=mkp->ibq; else pthread_barrier_wait(mkp->b); return NULL; } /**************************************************************/ /************ The writer *************/ /**************************************************************/ static void mkprof_write(struct mkprofparams *p) { double sum; char *jobname; struct timeval t1; gal_data_t *out=p->out, *log; struct builtqueue *ibq=NULL, *tbq; size_t complete=0, num=p->num, clog; /* Write each image into the output array. */ while(complete<p->num) { /* Set ibq. */ if(ibq==NULL) { if(p->cp.numthreads==1) ibq=p->bq; else { pthread_mutex_lock(&p->qlock); while(p->bq==NULL) pthread_cond_wait(&p->qready, &p->qlock); ibq=p->bq; p->bq=NULL; pthread_mutex_unlock(&p->qlock); } } sum=0.0f; /* During the build process, we also defined the overlap tiles of both the individual array and the final merged array, here we will use those to put the required profile pixels into the final array. */ if(ibq->overlaps && out) GAL_TILE_PO_OISET(float,float,ibq->overlap_i,ibq->overlap_m,1,0, { *o = p->replace ? ( *i==0.0f ? *o : *i ) : (*i + *o); sum += *i; }); /* Fill the log array. */ if(p->cp.log) { clog=0; for(log=p->log; log!=NULL; log=log->next) switch(++clog) { case 5: ((unsigned char *)(log->array))[ibq->id] = ibq->indivcreated; break; case 4: ((float *)(log->array))[ibq->id] = ibq->accufrac; break; case 3: ((unsigned long *)(log->array))[ibq->id]=ibq->numaccu; break; case 2: ((float *)(log->array))[ibq->id] = sum>0.0f ? -2.5f*log10(sum)+p->zeropoint : NAN; break; case 1: ((unsigned long *)(log->array))[ibq->id]=ibq->id+1; break; } } /* Report if in verbose mode. */ ++complete; if(!p->cp.quiet && p->num>1) { asprintf(&jobname, "row %zu complete, %zu left to go", ibq->id+1, num-complete); gal_timing_report(NULL, jobname, 2); free(jobname); } /* Free the array and the queue element and change it to the next one and increment complete. Note that there is no problem to free a NULL pointer (when the built array didn't overlap). */ gal_data_free(ibq->overlap_i); gal_data_free(ibq->overlap_m); gal_data_free(ibq->image); tbq=ibq->next; free(ibq); ibq=tbq; } /* Write the final array to the output FITS image if a merged image is to be created. */ if(out) { /* Get the current time for verbose output. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); /* Write the final image into a FITS file with the requested type. Until now, we were using `p->wcs' for the WCS, but from now on, will put it in `out' to also free it while freeing `out'. */ out->wcs=p->wcs; gal_fits_img_write_to_type(out, p->mergedimgname, NULL, PROGRAM_NAME, p->cp.type); p->wcs=NULL; /* Clean up */ gal_data_free(out); /* In verbose mode, print the information. */ if(!p->cp.quiet) { asprintf(&jobname, "%s created.", p->mergedimgname); gal_timing_report(&t1, jobname, 1); free(jobname); } } } /**************************************************************/ /************ Outside function *************/ /**************************************************************/ void mkprof(struct mkprofparams *p) { int err; char *tmp; pthread_t t; /* Thread id not used, all are saved here. */ pthread_attr_t attr; pthread_barrier_t b; struct mkonthread *mkp; gal_list_str_t *comments=NULL; size_t i, fi, *indexs, thrdcols; long *onaxes=NULL, os=p->oversample; size_t nb, ndim=p->ndim, nt=p->cp.numthreads; /* Allocate the arrays to keep the thread and parameters for each thread. Note that we only want nt-1 threads to do the building. */ errno=0; mkp=malloc(nt*sizeof *mkp); if(mkp==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `mkp'", __func__, (nt-1)*sizeof *mkp); /* Distribute the different profiles for different threads. Note that one thread is left out for writing, while nt-1 are left for building. */ gal_threads_dist_in_threads(p->num, nt, &indexs, &thrdcols); /* `onaxes' are size of the merged output image without over-sampling or shifting in FITS order. When no output merged image is needed, we can ignore it. */ if(p->out) { onaxes=gal_data_malloc_array(GAL_TYPE_LONG, ndim, __func__, "onaxes"); for(fi=0; fi < ndim; ++fi) { i=ndim-fi-1; onaxes[fi] = ( ( p->dsize[i] - 2 * p->shift[i] ) / os + 2 * p->shift[i]/os ); } } /* Build the profiles: */ if(nt==1) { mkp[0].p=p; mkp[0].onaxes=onaxes; mkp[0].indexs=indexs; mkp[0].rng=gsl_rng_clone(p->rng); mkprof_build(&mkp[0]); } else { /* Initialize the attributes. Note that this main thread will also have to be kept behind the barrier, so we need nt+1 barrier stops. */ if(p->num<nt) nb=p->num+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Initialize the condition variable and mutex. */ err=pthread_mutex_init(&p->qlock, NULL); if(err) error(EXIT_FAILURE, 0, "%s: mutex not initialized", __func__); err=pthread_cond_init(&p->qready, NULL); if(err) error(EXIT_FAILURE, 0, "%s: condition variable not initialized", __func__); /* Spin off the threads: */ for(i=0;i<nt;++i) if(indexs[i*thrdcols]!=GAL_BLANK_SIZE_T) { mkp[i].p=p; mkp[i].b=&b; mkp[i].ibq=NULL; mkp[i].onaxes=onaxes; mkp[i].rng=gsl_rng_clone(p->rng); mkp[i].indexs=&indexs[i*thrdcols]; err=pthread_create(&t, &attr, mkprof_build, &mkp[i]); if(err) error(EXIT_FAILURE, 0, "%s: can't create thread %zu", __func__, i); } } /* Write the created arrays into the image. */ mkprof_write(p); /* Write the log file. */ if(p->cp.log) { asprintf(&tmp, "Zeropoint: %g", p->zeropoint); gal_list_str_add(&comments, tmp, 0); gal_checkset_writable_remove(LOGFILENAME, 0, p->cp.dontdelete); gal_table_write_log(p->log, PROGRAM_STRING, &p->rawtime, comments, LOGFILENAME, p->cp.quiet); gal_list_str_free(comments, 1); } /* If numthreads>1, then wait for all the jobs to finish and destroy the attribute and barrier. */ if(nt>1) { pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); pthread_cond_destroy(&p->qready); pthread_mutex_destroy(&p->qlock); } /* Clean up. */ free(mkp); free(indexs); if(onaxes) free(onaxes); } ������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/ui.c������������������������������������������������������������������������0000644�0001750�0001750�00000137656�13216276304�013016� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/wcs.h> #include <gnuastro/box.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/table.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/tableintern.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "oneprofile.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "[Options] [Catalog]"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will create a FITS image " "containing any number of mock astronomical profiles based on an input " "catalog. All the profiles will be built from the center outwards. First " "by Monte Carlo integration, then using the central pixel position. The " "tolerance level specifies when the switch will occur.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static uint8_t ui_profile_name_read(char *string, size_t row) { if( !strcmp("sersic", string) ) return PROFILE_SERSIC; else if ( !strcmp("moffat", string) ) return PROFILE_MOFFAT; else if ( !strcmp("gaussian", string) ) return PROFILE_GAUSSIAN; else if ( !strcmp("point", string) ) return PROFILE_POINT; else if ( !strcmp("flat", string) ) return PROFILE_FLAT; else if ( !strcmp("circum", string) ) return PROFILE_CIRCUMFERENCE; else if ( !strcmp("distance", string) ) return PROFILE_DISTANCE; else if ( !strcmp(GAL_BLANK_STRING, string) ) error(EXIT_FAILURE, 0, "atleast one profile function is blank"); else { if(row) error(EXIT_FAILURE, 0, "`%s' not recognized as a profile function " "name in row %zu", string, row); else error(EXIT_FAILURE, 0, "`%s' not recognized as a profile function " "name in values to `--kernel' option", string); } return PROFILE_INVALID; } static char * ui_profile_name_write(int profile_code) { switch(profile_code) { case PROFILE_SERSIC: return "sersic"; case PROFILE_MOFFAT: return "moffat"; case PROFILE_GAUSSIAN: return "gaussian"; case PROFILE_POINT: return "point"; case PROFILE_FLAT: return "flat"; case PROFILE_CIRCUMFERENCE: return "circum"; case PROFILE_DISTANCE: return "distance"; default: error(EXIT_FAILURE, 0, "%s: %d not recognized as a profile code", __func__, profile_code); } return NULL; } static void ui_initialize_options(struct mkprofparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->poptions = program_options; cp->numthreads = gal_threads_number(); cp->coptions = gal_commonopts_options; /* Default program parameters. */ p->zeropoint = NAN; p->cp.type = GAL_TYPE_FLOAT32; /* Modify the common options for this program. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: cp->coptions[i].doc="Input catalog HDU name or number (if FITS)."; break; case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; break; case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct mkprofparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->catname) argp_error(state, "only one argument (input catalog) may be given"); else p->catname=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /* Parse the kernel properties, the format is like this: PROFILE_NAME,PARAM_1,PARAM_2,PARAM_3,...,PARAM_N */ void * ui_parse_kernel(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { long profcode; double *darray; gal_data_t *kernel; size_t i, nc, need=0; char *c, *profile, *tailptr; char *str, sstr[GAL_OPTIONS_STATIC_MEM_FOR_VALUES]; /* We want to print the stored values. */ if(lineno==-1) { /* Set the value pointer to kernel. */ kernel=*(gal_data_t **)(option->value); darray = kernel->array; /* First write the profile function code into the output string. */ nc=0; profile=ui_profile_name_write(kernel->status); nc += sprintf(sstr+nc, "%s,", profile); /* Write the values into a string. */ for(i=0;i<kernel->size;++i) { if( nc > GAL_OPTIONS_STATIC_MEM_FOR_VALUES-100 ) error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so we " "can address the problem. The number of necessary " "characters in the statically allocated string has become " "too close to %d", __func__, PACKAGE_BUGREPORT, GAL_OPTIONS_STATIC_MEM_FOR_VALUES); nc += sprintf(sstr+nc, "%g,", darray[i]); } sstr[nc-1]='\0'; /* Copy the string into a dynamically allocated space, because it will be freed later.*/ gal_checkset_allocate_copy(sstr, &str); return str; } else { /* The first part of `arg' (before the first comma) is not necessarily a number. So we need to separate the first part from the rest.*/ c=arg;while(*c!='\0' && *c!=',') ++c; profile=arg; arg = (*c=='\0') ? NULL : c+1; /* the `point' profile doesn't need */ *c='\0'; /* any numbers. */ /* Read the parameters. */ kernel=gal_options_parse_list_of_numbers(arg, filename, lineno); *(gal_data_t **)(option->value) = kernel; /* All parameters must be positive. */ darray=kernel->array; for(i=0;i<kernel->size;++i) if(darray[i]<=0) error(EXIT_FAILURE, 0, "value number %zu (%g) in the given list " "of kernel parameters (`%s') is not acceptable. All " "parameters to the `--kernel' option must be non-zero and " "positive", i+1, darray[i], arg); /* Write the profile type code into `kernel->status'. If it starts with a digit, then the user might have given the code of the profile directly. In that case, parse the number. Otherwise, let `ui_profile_name_read' find the value. */ if( isdigit(*profile) ) { profcode=strtol(profile, &tailptr, 0); if(*tailptr!='\0') error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' " "couldn't be read as a profile code", profile); if(profcode<=0 || profcode>=PROFILE_MAXIMUM_CODE) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' " "isn't a valid profile code. Please run with " "`--help' and see the acceptable codes in " "explanation of the `--fcol' option", profile); kernel->status=profcode; } else kernel->status=ui_profile_name_read(profile, 0); /* Make sure the number of parameters conforms with the profile. */ switch(kernel->status) { case PROFILE_SERSIC: need = 3; break; case PROFILE_MOFFAT: need = 3; break; case PROFILE_GAUSSIAN: need = 2; break; case PROFILE_POINT: need = 0; break; case PROFILE_FLAT: need = 1; break; case PROFILE_CIRCUMFERENCE: need = 1; break; case PROFILE_DISTANCE: need = 1; break; default: error_at_line(EXIT_FAILURE, 0, filename, lineno, "%s: a bug! " "Please contact us at %s to correct the issue. " "Profile code %d is not recognized", __func__, PACKAGE_BUGREPORT, kernel->status); } /* Make sure the number of parameters given are the same number that are needed. */ if( kernel->size != need ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "as a kernel, " "a `%s' profile needs %zu parameters, but %zu " "parameter%s given to `--kernel'", ui_profile_name_write(kernel->status), need, kernel->size, kernel->size>1?"s are":" is"); /* Our job is done, return NULL. */ return NULL; } } /* Parse the mode to interpret the given coordinates. */ void * ui_parse_coordinate_mode(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { char *outstr; /* We want to print the stored values. */ if(lineno==-1) { gal_checkset_allocate_copy( *(uint8_t *)(option->value)==MKPROF_MODE_IMG ? "img" : "wcs", &outstr ); return outstr; } else { if(!strcmp(arg, "img")) *(uint8_t *)(option->value)=MKPROF_MODE_IMG; else if (!strcmp(arg, "wcs")) *(uint8_t *)(option->value)=MKPROF_MODE_WCS; else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' (value to " "`--mode') not recognized as a coordinate standard " "mode. Recognized values are `img' and `wcs'. This " "option is necessary to identify the nature of your " "input coordinates", arg); return NULL; } } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct mkprofparams *p) { size_t i; /* When a no-merged image is to be created, type is necessary. */ if( p->cp.type==GAL_TYPE_INVALID && p->nomerged==0) error(EXIT_FAILURE, 0, "an output type `--type' is necessary when a " "merged image is to be built."); /* Check if one of the coordinate columns has been given, the other is also given. To simplify the job, we use the fact that conditions in C return either a 0 (when failed) and 1 (when successful). Note that if neighter coordinates are specified there is no problem, the user might have input the other coordinate standard. We'll also check for that after this.*/ if(p->kernel==NULL) { if(p->mode==0) error(EXIT_FAILURE, 0, "the `--mode' option is necessary when " "building profiles from a catalog. It can take two values: " "`img' or `wcs' which specify how to interpret the " "coordinate columns"); } /* The zeropoint magnitude is only necessary when `mcolisbrightness' is not called. */ if( p->mcolisbrightness==0 && isnan(p->zeropoint) ) error(EXIT_FAILURE, 0, "no zeropoint magnitude given. A zeropoint " "magnitude is necessary when `--mcolisbrightness' is not called " "(i.e., when the contents of `--mcol' must be interpretted as " "a magnitude, not brightness)."); /* Make sure no zero value is given for the `--naxis' option (only when it is necessary). */ if(p->dsize && p->backname==NULL) for(i=0;p->dsize[i]!=GAL_BLANK_SIZE_T;++i) if(p->dsize[i]==0) error(EXIT_FAILURE, 0, "values to `--naxes' option must not be " "zero"); } /* Sanity check on options AND arguments. If only option values are to be checked, use `ui_read_check_only_options'. */ static void ui_check_options_and_arguments(struct mkprofparams *p) { int d0f1; char *tmpname; /* If no kernel is given, make sure an input catalog is given, and if it is FITS, that the HDU is also provided. When a kernel option, we will set a fiducial catalog name called `kernel.txt' to automatic output filename generation. */ if(p->kernel) { if(p->catname) error(EXIT_FAILURE, 0, "`--kernel' cannot be called with an input " "catalog (`%s'). The parameters necessary to build a single " "kernel output should be given to `--kernel', not in a " "catalog", p->catname); p->catname="kernel.option"; } else { if(p->catname) { if( gal_fits_name_is_fits(p->catname) && p->cp.hdu==NULL) error(EXIT_FAILURE, 0, "no `hdu' specified for the input FITS " "table '%s', to ", p->catname); } else error(EXIT_FAILURE, 0, "no input catalog provided. To build " "profiles, you need to give a catalog/table containing " "the information of the profiles"); } /* If cp->output was not specified on the command line or in any of the configuration files, then automatic output should be used, in which case, cp->output should be the current directory. */ if(p->cp.output==NULL) gal_checkset_allocate_copy("./", &p->cp.output); /* Set the necessary output names. */ d0f1=gal_checkset_dir_0_file_1(p->cp.output, p->cp.dontdelete); if(d0f1) /* --output is a file name. */ { p->mergedimgname=p->cp.output; p->outdir=gal_checkset_dir_part(p->mergedimgname); } else /* --output is a directory name. */ { gal_checkset_allocate_copy(p->cp.output, &p->outdir); gal_checkset_check_dir_write_add_slash(&p->outdir); tmpname=gal_checkset_automatic_output(&p->cp, p->catname, ".fits"); p->mergedimgname=gal_checkset_malloc_cat(p->outdir, tmpname); free(tmpname); } p->basename=gal_checkset_not_dir_part(p->mergedimgname); /* If a merged image is requested (or `--kernel' the option is called), then delete the final filename if it exists. */ if(p->nomerged==0 && p->kernel) gal_checkset_writable_remove(p->mergedimgname, p->cp.keep, p->cp.dontdelete); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ static void ui_read_cols(struct mkprofparams *p) { int checkblank; size_t i, counter=0; char *colname=NULL, **strarr; gal_list_str_t *colstrs=NULL, *ccol; gal_data_t *cols, *tmp, *corrtype=NULL; /* The coordinate columns are a linked list of strings. */ ccol=p->ccol; for(i=0; i<p->ndim; ++i) { gal_list_str_add(&colstrs, ccol->v, 0); ccol=ccol->next; } /* Add the rest of the columns in a specific order. */ gal_list_str_add(&colstrs, p->fcol, 0); gal_list_str_add(&colstrs, p->rcol, 0); gal_list_str_add(&colstrs, p->ncol, 0); gal_list_str_add(&colstrs, p->pcol, 0); gal_list_str_add(&colstrs, p->qcol, 0); gal_list_str_add(&colstrs, p->mcol, 0); gal_list_str_add(&colstrs, p->tcol, 0); /* Reverse the order to make the column orders correspond to how we added them here and avoid possible bugs. */ gal_list_str_reverse(&colstrs); /* Read the desired columns from the file. */ cols=gal_table_read(p->catname, p->cp.hdu, colstrs, p->cp.searchin, p->cp.ignorecase, p->cp.minmapsize, NULL); /* Set the number of objects. */ p->num=cols->size; /* Put each column's data in the respective internal array. */ while(cols!=NULL) { /* Pop out the top column. */ tmp=gal_list_data_pop(&cols); /* By default check if the column has blank values, but it can be turned off for some columns. */ checkblank=1; /* See which column we are currently reading. */ switch(++counter) { case 1: case 2: colname = ( counter==1 ? "first coordinate column (`--coordcol')" : "second coordinate column (`--coordcol')" ); corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT64); switch(counter) { case 1: p->x=corrtype->array; break; case 2: p->y=corrtype->array; break; } break; case 3: if(tmp->type==GAL_TYPE_STRING) { p->f=gal_data_malloc_array(GAL_TYPE_UINT8, p->num, __func__, "p->f"); strarr=tmp->array; for(i=0;i<p->num;++i) p->f[i]=ui_profile_name_read(strarr[i], i+1); gal_data_free(tmp); corrtype=NULL; } else { /* Read the user's profile codes. */ colname="profile function code (`fcol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_UINT8); p->f=corrtype->array; /* Check if they are in the correct range. */ for(i=0;i<p->num;++i) if(p->f[i]<=PROFILE_INVALID || p->f[i]>=PROFILE_MAXIMUM_CODE) error(EXIT_FAILURE, 0, "%s: row %zu, the function " "code is %u. It should be >%d and <%d. Please run " "again with `--help' and check the acceptable " "codes.\n\nAlternatively, you can use alphabetic " "strings to specify the profile functions, see the " "explanations under `fcol' from the command " "below (press the `SPACE' key to go down, and the " "`q' to return back to the command-line):\n\n" " $ info %s\n", p->catname, i+1, p->f[i], PROFILE_INVALID, PROFILE_MAXIMUM_CODE, PROGRAM_EXEC); } break; case 4: colname="radius (`rcol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->r=corrtype->array; /* Check if there is no negative or zero-radius profile. */ for(i=0;i<p->num;++i) if(p->r[i]<=0.0f) error(EXIT_FAILURE, 0, "%s: row %zu, the radius value %g is " "not acceptable. It has to be larger than 0", p->catname, i+1, p->r[i]); break; case 5: colname="index (`ncol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->n=corrtype->array; break; case 6: colname="position angle (`pcol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->p=corrtype->array; break; case 7: colname="axis ratio (`qcol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->q=corrtype->array; /* Check if there is no negative or >1.0f axis ratio. */ for(i=0;i<p->num;++i) if(p->q[i]<=0.0f || p->q[i]>1.0f) error(EXIT_FAILURE, 0, "%s: row %zu, the axis ratio value %g " "is not acceptable. It has to be >0 and <=1", p->catname, i+1, p->q[i]); break; case 8: colname="magnitude (`mcol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->m=corrtype->array; checkblank=0; /* Magnitude can be NaN: to mask regions. */ break; case 9: colname="truncation (`tcol')"; corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT32); p->t=corrtype->array; /* Check if there is no negative or zero truncation radius. */ for(i=0;i<p->num;++i) if(p->t[i]<=0.0f) error(EXIT_FAILURE, 0, "%s: row %zu, the truncation radius " "value %g is not acceptable. It has to be larger than 0", p->catname, i+1, p->t[i]); break; /* If the index isn't recognized, then it is larger, showing that there was more than one match for the given criteria */ default: gal_tableintern_error_col_selection(p->catname, p->cp.hdu, "too " "many columns were selected " "by the given values to the " "options ending in `col'."); } /* Sanity check and clean up. Note that it might happen that the input structure is already freed. In that case, `corrtype' will be NULL. */ if(corrtype) { /* Make sure there are no blank values in this column. */ if( checkblank && gal_blank_present(corrtype, 1) ) error(EXIT_FAILURE, 0, "%s column has blank values. " "Input columns cannot contain blank values", colname); /* Free the unnecessary sturcture information. The correct-type (`corrtype') data structure's array is necessary for later steps, so its pointer has been copied in the main program's structure. Hence, we should set the structure's pointer to NULL so the important data isn't freed.*/ corrtype->array=NULL; gal_data_free(corrtype); } } } /* It is possible to define the internal catalog through a catalog or the `--kernel' option. This function will do the job. */ static void ui_prepare_columns(struct mkprofparams *p) { double *karr; float r, n, t; /* If the kernel option was called, then we need to build a series of single element columns to create an internal catalog. */ if(p->kernel) { /* Number of profiles to be built. */ p->num=1; /* Allocate the necessary columns. */ p->x = gal_data_calloc_array(GAL_TYPE_FLOAT64, 1, __func__, "p->x"); p->y = gal_data_calloc_array(GAL_TYPE_FLOAT64, 1, __func__, "p->y"); p->f = gal_data_calloc_array(GAL_TYPE_UINT8, 1, __func__, "p->f"); p->r = gal_data_calloc_array(GAL_TYPE_FLOAT32, 1, __func__, "p->r"); p->n = gal_data_calloc_array(GAL_TYPE_FLOAT32, 1, __func__, "p->n"); p->p = gal_data_calloc_array(GAL_TYPE_FLOAT32, 1, __func__, "p->p"); p->q = gal_data_calloc_array(GAL_TYPE_FLOAT32, 1, __func__, "p->q"); p->m = gal_data_calloc_array(GAL_TYPE_FLOAT32, 1, __func__, "p->m"); p->t = gal_data_calloc_array(GAL_TYPE_FLOAT32, 1, __func__, "p->t"); /* For profiles that need a different number of input values. Note that when a profile doesn't need a value, it will be ignored. */ karr=p->kernel->array; if(p->kernel->size) { r = karr[0]; n = p->kernel->size==2 ? 0.0f : karr[1]; t = p->kernel->size==1 ? 1.0f : karr[ p->kernel->size - 1 ]; } else r=n=t=0.0f; /* Fill the allocated spaces. */ p->x[0] = 0.0f; p->y[0] = 0.0f; p->f[0] = p->kernel->status; p->r[0] = r; p->n[0] = n; p->p[0] = 0.0f; p->q[0] = 1.0f; p->m[0] = 0.0f; p->t[0] = t; } else { /* Make sure the number of coordinate columns and number of dimensions in outputs are the same. There is no problem if it is more than `ndim'. In that case, the last values (possibly in configuration files) will be ignored. */ if( gal_list_str_number(p->ccol) < p->ndim ) error(EXIT_FAILURE, 0, "%zu coordinate columns (calls to " "`--coordcol') given but output has %zu dimensions", gal_list_str_number(p->ccol), p->ndim); /* Call the column-reading function. */ ui_read_cols(p); } } /* To keep things clean, we'll do the WCS sanity checks in this small function. If everything is ok, this function will return 0 (so an if condition won't be executed). If any of the necessary inputs aren't given, it will return 1. */ static int ui_wcs_sanity_check(struct mkprofparams *p) { size_t ndim=p->ndim; if(p->crpix) { if(p->crpix->size!=ndim) error(EXIT_FAILURE, 0, "%zu values given to `--crpix'. This must be " "the same as the output dimension (%zu)", p->crpix->size, ndim); return 0; } else return 1; if(p->crval) { if(p->crval->size!=ndim) error(EXIT_FAILURE, 0, "%zu values given to `--crval'. This must be " "the same as the output dimension (%zu)", p->crval->size, ndim); return 0; } else return 1; if(p->cdelt) { if(p->cdelt->size!=ndim) error(EXIT_FAILURE, 0, "%zu values given to `--cdelt'. This must be " "the same as the output dimension (%zu)", p->cdelt->size, ndim); return 0; } else return 1; if(p->pc) { if(p->pc->size!=ndim*ndim) error(EXIT_FAILURE, 0, "%zu values given to `--pc'. This must be " "the square as the output dimension (%zu)", p->pc->size, ndim*ndim); return 0; } else return 1; if(p->cunit) { if(p->cunit->size!=ndim) error(EXIT_FAILURE, 0, "%zu values given to `--cunit'. This must be " "the same as the output dimension (%zu)", p->cunit->size, ndim); return 0; } else return 1; if(p->ctype) { if(p->ctype->size!=ndim) error(EXIT_FAILURE, 0, "%zu values given to `--ctype'. This must be " "the same as the output dimension (%zu)", p->ctype->size, ndim); return 0; } else return 1; } static void ui_prepare_wcs(struct mkprofparams *p) { int status; struct wcsprm *wcs; char **cunit, **ctype; size_t i, ndim=p->ndim; double *crpix, *crval, *cdelt, *pc; /* Check and initialize the WCS information. If any of the necessary WCS parameters are missing, then don't build any WCS. */ if( ui_wcs_sanity_check(p) ) return; crpix = p->crpix->array; crval = p->crval->array; cdelt = p->cdelt->array; pc = p->pc->array; cunit = p->cunit->array; ctype = p->ctype->array; /* Allocate the memory necessary for the wcsprm structure. */ errno=0; wcs=p->wcs=malloc(sizeof *wcs); if(wcs==NULL) error(EXIT_FAILURE, errno, "%zu for wcs in preparewcs", sizeof *wcs); /* Initialize the structure (allocate all its internal arrays). */ wcs->flag=-1; if( (status=wcsini(1, ndim, wcs)) ) error(EXIT_FAILURE, 0, "wcsini error %d: %s", status, wcs_errmsg[status]); /* Fill in all the important WCS structure parameters. */ wcs->altlin = 0x1; wcs->equinox = 2000.0f; for(i=0;i<ndim;++i) { /* IMPORTANT: At this point, we don't want the WCS to be over-sampled because if the user has given RA and Dec for the profiles, they need to be converted to non-oversampled and shifted image coordinates. After the conversion (in `ui_finalize_coordinates') we are going to correct for the oversampling in the WCS.*/ wcs->crpix[i] = crpix[i]; wcs->crval[i] = crval[i]; wcs->cdelt[i] = cdelt[i]; strcpy(wcs->cunit[i], cunit[i]); strcpy(wcs->ctype[i], ctype[i]); } for(i=0;i<ndim*ndim;++i) wcs->pc[i]=pc[i]; /* Set up the wcs structure with the constants defined above. */ status=wcsset(wcs); if(status) error(EXIT_FAILURE, 0, "wcsset error %d: %s", status, wcs_errmsg[status]); } static void ui_prepare_canvas(struct mkprofparams *p) { float *f, *ff; double truncr; gal_data_t *keysll; long width[2]={1,1}; int status=0, setshift=0; size_t i, nshift=0, *dsize=NULL, ndim_counter; /* If a background image is specified, then use that as the output image to build the profiles over. */ if(p->backname) { /* Make sure the kernel option is not called. */ if(p->kernel) error(EXIT_FAILURE, 0, "the `--kernel' and `--background' options " "cannot be called together"); /* Small sanity check. */ if(p->backhdu==NULL) error(EXIT_FAILURE, 0, "no hdu specified for the background image " "%s. Please run again `--backhdu' option", p->backname); /* Read in the background image and its coordinates, note that when no merged image is desired, we just need the WCS information of the background image and the number of its dimensions. So `ndim==0' and what `dsize' points to is irrelevant. */ if(p->nomerged) { /* Get the number of the background image's dimensions. */ keysll=gal_data_array_calloc(1); keysll->name="NAXIS"; keysll->type=GAL_TYPE_SIZE_T; gal_fits_key_read(p->backname, p->backhdu, keysll, 0, 0); p->ndim = *(size_t *)(keysll->array); keysll->name=NULL; gal_data_array_free(keysll, 1, 1); /* Read the WCS structure of the background image. */ p->wcs=gal_wcs_read(p->backname, p->backhdu, 0, 0, &p->nwcs); } else { /* Read the image. */ p->out=gal_fits_img_read_to_type(p->backname, p->backhdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0, 0); /* Put the WCS structure and number of dimensions in the MakeProfiles's main structure for generality. The WCS structure will be put back in the end when writing. */ p->wcs=p->out->wcs; p->nwcs=p->out->nwcs; p->ndim=p->out->ndim; p->out->wcs=NULL; p->out->nwcs=0; /* If p->dsize was given as an option, free it. */ if( p->dsize ) free(p->dsize); /* Write the size of the background image into `dsize'. */ p->dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, p->ndim, __func__, "p->dsize"); for(i=0;i<p->ndim;++i) p->dsize[i] = p->out->dsize[i]; /* Set all pixels to zero if the user wanted a clear canvas. */ if(p->clearcanvas) {ff=(f=p->out->array)+p->out->size; do *f++=0.0f; while(f<ff);} } /* Currently, things are only implemented for 2D. */ if(p->ndim!=2) error(EXIT_FAILURE, 0, "%s (hdu %s) has %zu dimensions. Currently " "only a 2 dimensional background image is acceptable", p->backname, p->backhdu, p->ndim); /* When a background image is specified, oversample must be 1 and there is no shifts. */ p->oversample=1; if(p->shift) free(p->shift); p->shift=gal_data_calloc_array(GAL_TYPE_SIZE_T, p->ndim, __func__, "p->shift (1)"); } else { /* Get the number of dimensions. */ ndim_counter=0; for(i=0;p->dsize[i]!=GAL_BLANK_SIZE_T;++i) ++ndim_counter; p->ndim=ndim_counter; /* Currently, things are only implemented for 2D. */ if(p->ndim!=2) error(EXIT_FAILURE, 0, "%zu numbers given to `--naxis', only 2 " "values may be given", p->ndim); /* If any of the shift elements are zero, the others should be too!*/ if(p->shift && p->shift[0] && p->shift[1]) { /* Multiply the shift by the over-sample. */ for(i=0;p->shift[i]!=GAL_BLANK_SIZE_T;++i) { ++nshift; p->shift[i] *= p->oversample; } /* Make sure it has the same number of elements as naxis. */ if(p->ndim!=nshift) error(EXIT_FAILURE, 0, "%zu and %zu elements given to `--ndim' " "and `--shift' respectively. These two numbers must be the " "same", p->ndim, nshift); } else { /* `prepforconv' is only valid when xshift and yshift are both zero. Also, a PSF profile should exist in the image. */ if(p->prepforconv) { /* Check if there is at least one Moffat or Gaussian profile. */ for(i=0;i<p->num;++i) if( oneprofile_ispsf(p->f[i]) ) { /* Calculate the size of the box holding the PSF. Note: - For the Moffat and Gaussian profiles, the radius column is actually the FWHM which is actually the diameter, not radius. So we have to divide it by half. - encloseellipse outputs the total width, we only want half of it for the shift. */ setshift=1; truncr = p->tunitinp ? p->t[i] : p->t[i] * p->r[i]/2; gal_box_bound_ellipse(truncr, p->q[i]*truncr, p->p[i], width); } /* Either set the shifts to zero or to the values set from the PSF. Note that the user might have given any number of shifts (from zero). So, we'll just free it and reset it. */ if(p->shift) free(p->shift); p->shift=gal_data_calloc_array(GAL_TYPE_SIZE_T, p->ndim, __func__, "p->shift (2)"); if(setshift) { p->shift[0] = (width[0]/2)*p->oversample; p->shift[1] = (width[1]/2)*p->oversample; } } } /* If shift has not been set until now, set it. */ if(p->shift==NULL) p->shift=gal_data_calloc_array(GAL_TYPE_SIZE_T, p->ndim, __func__, "p->shift (3)"); /* Prepare the sizes of the final merged image (if it is to be made). Note that even if we don't want a merged image, we still need its WCS structure. */ if(p->nomerged==0) { ndim_counter=0; for(i=0;p->dsize[i]!=GAL_BLANK_SIZE_T;++i) { /* Count the number of dimensions. */ ++ndim_counter; /* Correct dsize. */ p->dsize[i] = (p->dsize[i]*p->oversample) + (2*p->shift[i]); } dsize = p->dsize; /* Make the output structure. */ p->out=gal_data_alloc(NULL, GAL_TYPE_FLOAT32, ndim_counter, dsize, NULL, 1, p->cp.minmapsize, NULL, NULL, NULL); } } /* Make the WCS structure of the output data structure if it has not been set yet. */ if(p->wcs==NULL) ui_prepare_wcs(p); /* Set the name, comments and units of the final merged output. */ if(p->out) { if(p->out->name) free(p->out->name); gal_checkset_allocate_copy("Mock profiles", &p->out->name); if(p->out->unit==NULL) gal_checkset_allocate_copy("Brightness", &p->out->unit); } /* When individual mode is requested, write the WCS structure to a header string to speed up the process: if we don't do it here, this process will be necessary on every individual profile's output. So it is much more efficient done once here. */ if(p->individual && p->wcs) { status=wcshdo(WCSHDO_safe, p->wcs, &p->wcsnkeyrec, &p->wcsheader); if(status) error(EXIT_FAILURE, 0, "wcshdo error %d: %s", status, wcs_errmsg[status]); } } static void ui_finalize_coordinates(struct mkprofparams *p) { void *arr=NULL; size_t i=0, ndim=p->ndim; uint8_t os=p->oversample; gal_data_t *tmp, *coords=NULL; double *cdelt=p->wcs->cdelt, *crpix=p->wcs->crpix; /* When the user specified RA and Dec columns, the respective values where stored in the `p->x' and `p->y' arrays. So before proceeding, we need to change them into actual image coordinates. */ if(p->mode==MKPROF_MODE_WCS) { /* Make list of coordinates for input of `gal_wcs_world_to_img'. */ for(i=0;i<ndim;++i) { /* Set the array pointer. Note that we read the WCS columns into the `p->x', `p->y' and `p->z' arrays temporarily before. Here, we will convert them to image coordinates in place. */ switch(i) { /* Note that the linked list gets filled in a first-in-last-out order, so the last column added should be the first WCS dimension. */ case 0: arr = p->y; break; case 1: arr = p->x; break; default: error(EXIT_FAILURE, 0, "conversion from WCS to image " "coordinates is not currently supported for " "%zu-dimensional datasets", ndim); } /* Allocate the list of coordinates. */ gal_list_data_add_alloc(&coords, arr, GAL_TYPE_FLOAT64, 1, &p->num, NULL, 0, -1, NULL, NULL, NULL); } /* Convert the world coordinates to image coordinates (inplace). */ gal_wcs_world_to_img(coords, p->wcs, 1); /* If any conversions created a WCSLIB error, both the outputs will be set to NaN. */ for(i=0;i<p->num;++i) if( isnan(p->x[i]) ) error(EXIT_FAILURE, 0, "catalog row %zu: WCSLIB could not convert " "(%f, %f) coordinates into image coordinates", i, p->x[i], p->y[i]); /* We want the actual arrays of each `coords' column. So, first we'll set all the array elements to NULL, then free it. */ for(tmp=coords;tmp!=NULL;tmp=tmp->next) tmp->array=NULL; gal_list_data_free(coords); } /* Correct the WCS scale. Note that when the WCS is read from a background image, oversample is set to 1. This is done here because the conversion of WCS to pixel coordinates needs to be done with the non-over-sampled image.*/ for(i=0;i<p->ndim;++i) { /* Oversampling has already been applied in `p->shift'. Also note that shift is in the C dimension ordring, while crpix is in FITS ordering. */ crpix[i] = crpix[i]*os + p->shift[ndim-i-1] - os/2; cdelt[i] /= os; } /* For a sanity check: printf("\nui_finalize_coordinates sanity check:\n"); for(i=0;i<p->num;++i) printf("%f, %f\n", p->x[i], p->y[i]); */ } /* Add all the columns of the log file. Just note that since this is a linked list, we have to add them in the opposite order. */ static void ui_make_log(struct mkprofparams *p) { char *name, *comment; /* Return if no long file is to be created. */ if(p->cp.log==0) return; /* Individual created. */ gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_UINT8, 1, &p->num, NULL, 1, p->cp.minmapsize, "INDIV_CREATED", "bool", "If an individual image was made (1) or not (0)."); /* Fraction of monte-carlo. */ gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_FLOAT32, 1, &p->num, NULL, 1, p->cp.minmapsize, "FRAC_MONTECARLO", "frac", "Fraction of brightness in Monte-carlo integrated " "pixels."); /* Number of monte-carlo. */ gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_UINT64, 1, &p->num, NULL, 1, p->cp.minmapsize, "NUM_MONTECARLO", "count", "Number of Monte Carlo integrated pixels."); /* Magnitude of profile overlap. */ gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_FLOAT32, 1, &p->num, NULL, 1, p->cp.minmapsize, "MAG_OVERLAP", "mag", "Magnitude of profile's overlap with merged " "image."); /* Row number in input catalog. */ name=gal_fits_name_save_as_string(p->catname, p->cp.hdu); asprintf(&comment, "Row number of profile in %s.", name); gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_UINT64, 1, &p->num, NULL, 1, p->cp.minmapsize, "INPUT_ROW_NO", "count", comment); free(comment); free(name); } static void ui_preparations(struct mkprofparams *p) { /* If the kernel option was given, some parameters need to be over-written: */ if(p->kernel) { /* Set the necessary constants. */ p->ndim=2; p->nomerged=1; p->psfinimg=0; p->individual=1; /* Set the shift array. */ p->shift=gal_data_calloc_array(GAL_TYPE_SIZE_T, p->ndim, __func__, "p->shift"); } else ui_prepare_canvas(p); /* Read in all the columns. */ ui_prepare_columns(p); /* Read the (possible) RA/Dec inputs into X and Y for the builder.*/ if(p->wcs) ui_finalize_coordinates(p); /* Allocate the random number generator: */ gsl_rng_env_setup(); p->rng=gsl_rng_alloc(gsl_rng_ranlxs1); /* Make the log linked list. */ ui_make_log(p); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ static void ui_print_intro(struct mkprofparams *p) { char *jobname; if(p->cp.quiet) return; printf(PROGRAM_NAME" started on %s", ctime(&p->rawtime)); if(p->kernel) asprintf(&jobname, "Building one %s kernel", ui_profile_name_write(p->kernel->status)); else asprintf(&jobname, "%zu profile%sread from %s", p->num, p->num>1?"s ":" ", p->catname); gal_timing_report(NULL, jobname, 1); free(jobname); if(p->backname) { if(p->nomerged) asprintf(&jobname, "WCS information read from %s", p->backname); else asprintf(&jobname, "%s is read and will be used as canvas", p->backname); gal_timing_report(NULL, jobname, 1); free(jobname); } asprintf(&jobname, "Random number generator (RNG) type: %s", gsl_rng_name(p->rng)); gal_timing_report(NULL, jobname, 1); free(jobname); if(p->envseed) { asprintf(&jobname, "RNG seed for all profiles: %lu", gsl_rng_default_seed); gal_timing_report(NULL, jobname, 1); free(jobname); } if(p->kernel==NULL) { asprintf(&jobname, "Using %zu threads.", p->cp.numthreads); gal_timing_report(NULL, jobname, 1); free(jobname); } } void ui_read_check_inputs_setup(int argc, char *argv[], struct mkprofparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the sanity check so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Print introductory information. */ ui_print_intro(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct mkprofparams *p, struct timeval *t1) { /* Free all the allocated arrays. */ free(p->cat); free(p->cp.hdu); free(p->outdir); free(p->basename); /* p->cp.output might be equal to p->mergedimgname. In this case, if we simply free them after each other, there will be a double free error. So after freeing output, we set it to NULL since free(NULL) is ok.*/ if(p->cp.output==p->mergedimgname) free(p->cp.output); else { free(p->cp.output); free(p->mergedimgname); } /* Free the WCS headers string that was defined for individual mode. */ if(p->individual) free(p->wcsheader); /* Free the random number generator: */ gsl_rng_free(p->rng); /* Free the log file information. */ if(p->cp.log) gal_list_data_free(p->log); /* Report the duration of the job */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in", 0); } ����������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/main.c����������������������������������������������������������������������0000644�0001750�0001750�00000003125�13121462410�013272� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeProfiles - Create mock astronomical profiles. MakeProfiles is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "mkprof.h" #include "ui.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct mkprofparams p={{{0},0},0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ mkprof(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/Makefile.in�����������������������������������������������������������������0000644�0001750�0001750�00000211666�13217217705�014275� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. 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GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for MakeProfiles. # MakeProfiles is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. 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This file is offered as-is, without any # warranty. #input backhdu 1 # Output: naxis 1000,1000 oversample 5 circumwidth 2 type float32 # Profiles: tunitinp 0 numrandom 10000 tolerance 0.01 zeropoint 0.00 # Catalog: mode img ccol 2 ccol 3 fcol 4 rcol 5 ncol 6 pcol 7 qcol 8 mcol 9 tcol 10 # WCS: crpix 1,1 crval 1,1 cdelt 0.03/3600,0.03/3600 pc -1,0,0,1 cunit deg,deg ctype RA---TAN,DEC--TAN ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkprof/Makefile.am�����������������������������������������������������������������0000644�0001750�0001750�00000002655�13216276304�014257� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astmkprof astmkprof_LDADD = -lgnuastro astmkprof_SOURCES = main.c ui.c mkprof.c oneprofile.c profiles.c EXTRA_DIST = main.h authors-cite.h args.h ui.h mkprof.h oneprofile.h \ profiles.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmkprof.conf �����������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/���������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220467�012442� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/mknoise.h������������������������������������������������������������������0000644�0001750�0001750�00000002047�12616616510�014203� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MKNOISE_H #define MKNOISE_H void mknoise(struct mknoiseparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/ui.h�����������������������������������������������������������������������0000644�0001750�0001750�00000003202�13174462540�013147� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Available letters for short options: a c d f g j k l m n p r t u v w x y A B C E G H J L O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_SIGMA = 's', UI_KEY_INSTRUMENTAL = 'i', UI_KEY_BACKGROUND = 'b', UI_KEY_ZEROPOINT = 'z', UI_KEY_ENVSEED = 'e', /* Only with long version (start with a value 1000, the rest will be set automatically). */ }; void ui_read_check_inputs_setup(int argc, char *argv[], struct mknoiseparams *p); void ui_free_report(struct mknoiseparams *p, struct timeval *t1); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/args.h���������������������������������������������������������������������0000644�0001750�0001750�00000006072�13136637645�013506� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { { "sigma", UI_KEY_SIGMA, "FLT", 0, "Total noise sigma, ignore other options.", GAL_OPTIONS_GROUP_INPUT, &p->sigma, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "instrumental", UI_KEY_INSTRUMENTAL, "FLT", 0, "Instrument noise level (in pixel value units).", GAL_OPTIONS_GROUP_INPUT, &p->instrumental, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "background", UI_KEY_BACKGROUND, "FLT", 0, "Fixed background magnitude for whole input.", GAL_OPTIONS_GROUP_INPUT, &p->background_mag, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "zeropoint", UI_KEY_ZEROPOINT, "FLT", 0, "Zeropoint magnitude of input.", GAL_OPTIONS_GROUP_INPUT, &p->zeropoint, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "envseed", UI_KEY_ENVSEED, 0, 0, "Use GSL_RNG_SEED environment variable for seed", GAL_OPTIONS_GROUP_OPERATING_MODE, &p->envseed, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/authors-cite.h�������������������������������������������������������������0000644�0001750�0001750�00000002752�13211076737�015153� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ����������������������gnuastro-0.5/bin/mknoise/main.h���������������������������������������������������������������������0000644�0001750�0001750�00000004662�13136637645�013501� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gsl/gsl_rng.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "MakeNoise" /* Program full name. */ #define PROGRAM_EXEC "astmknoise" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Main program parameters structure */ struct mknoiseparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ char *inputname; /* Input filename. */ double sigma; /* Total noise sigma (ignoring others). */ double instrumental; /* Standard deviation constants. */ double zeropoint; /* Zeropoint magnitude of image. */ double background_mag; /* Background in magnitudes. */ uint8_t envseed; /* ==1, generate a random seed. */ /* Internal */ gal_data_t *input; /* Input image data in double precision. */ double background; /* Background in units of brightness. */ gsl_rng *rng; /* Main instance of random number generator.*/ char *rng_type; /* The type of the Random number gen. */ int64_t rng_seed; /* Seed of Random number generator. */ time_t rawtime; /* Starting time of the program. */ }; #endif ������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/mknoise.c������������������������������������������������������������������0000644�0001750�0001750�00000007661�13151366335�014207� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <sys/time.h> /* Generate random seed. */ #include <gsl/gsl_rng.h> /* Used in setrandoms. */ #include <gnuastro/fits.h> #include <gsl/gsl_randist.h> /* To make noise. */ #include <gnuastro-internal/timing.h> #include "main.h" void convertsaveoutput(struct mknoiseparams *p) { char keyname1[FLEN_KEYWORD]; gal_fits_list_key_t *headers=NULL; char keyname2[FLEN_KEYWORD], keyname3[FLEN_KEYWORD]; char keyname4[FLEN_KEYWORD], keyname5[FLEN_KEYWORD]; /* Add the proper information to the header of the output: */ gal_fits_key_write_filename("INF", p->inputname, &headers); if( !isnan(p->background_mag) ) { strcpy(keyname1, "BCKGRND"); gal_fits_key_list_add_end(&headers, GAL_TYPE_FLOAT64, keyname1, 0, &p->background_mag, 0, "Background " "value (in magnitude) for noise.", 0, NULL); strcpy(keyname2, "BZRPNT"); gal_fits_key_list_add_end(&headers, GAL_TYPE_FLOAT64, keyname2, 0, &p->zeropoint, 0, "Zeropoint magnitude of image.", 0, NULL); strcpy(keyname3, "INSTRU"); gal_fits_key_list_add_end(&headers, GAL_TYPE_FLOAT64, keyname3, 0, &p->instrumental, 0, "Instrumental noise in units of flux.", 0, NULL); } else { strcpy(keyname1, "SIGMA"); gal_fits_key_list_add_end(&headers, GAL_TYPE_FLOAT64, keyname1, 0, &p->sigma, 0, "Total noise sigma", 0, NULL); } strcpy(keyname4, "RNGTYPE"); gal_fits_key_list_add_end(&headers, GAL_TYPE_STRING, keyname4, 0, p->rng_type, 0, "Random number generator (by " "GSL) type.", 0, NULL); strcpy(keyname5, "RNGSEED"); gal_fits_key_list_add_end(&headers, GAL_TYPE_INT64, keyname5, 0, &p->rng_seed, 0, "Random number generator (by GSL) seed.", 0, NULL); /* Save the output: */ p->input=gal_data_copy_to_new_type_free(p->input, p->cp.type); gal_fits_img_write(p->input, p->cp.output, headers, PROGRAM_NAME); } void mknoise(struct mknoiseparams *p) { double *d, *df, background=p->background, instrumental=p->instrumental; /* Add the noise: */ df=(d=p->input->array)+p->input->size; if( !isnan(p->sigma) ) { do *d += gsl_ran_gaussian(p->rng, p->sigma); while(++d<df); } else { do *d += ( background + gsl_ran_gaussian(p->rng, sqrt( instrumental + background + *d )) ); while(++d<df); } /* Convert and save the output in the proper format: */ convertsaveoutput(p); } �������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/ui.c�����������������������������������������������������������������������0000644�0001750�0001750�00000026754�13175670623�013167� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <inttypes.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/tableintern.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will add noise to all the " "pixels in an input dataset. The noise parameters can be specified with " "the options below. \n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct mknoiseparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->poptions = program_options; cp->coptions = gal_commonopts_options; /* Initialize options for this program. */ p->sigma = NAN; p->zeropoint = NAN; p->background_mag = NAN; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Selet individually */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct mknoiseparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->inputname) argp_error(state, "only one argument (input file) should be given"); else p->inputname=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct mknoiseparams *p) { /* At leaset one of `--sigma' or `--background' are necessary. */ if( isnan(p->sigma) && isnan(p->background_mag) ) error(EXIT_FAILURE, 0, "at least one of `--sigma' or `--background' " "must be given to identify the noise level"); /* If a background magnitude is given (and the user hasn't given a `--sigma'), the zeropoint is necessary. */ if( isnan(p->sigma) && !isnan(p->background_mag) && isnan(p->zeropoint) ) error(EXIT_FAILURE, 0, "no zeropoint magnitude given. When the noise is " "identified by the background magnitude, a zeropoint magnitude " "is mandatory. Please use the `--zeropoint' option to specify " "a zeropoint magnitude"); } static void ui_check_options_and_arguments(struct mknoiseparams *p) { /* Make sure an input file name was given and if it was a FITS file, that a HDU is also given. */ if(p->inputname) { if( gal_fits_name_is_fits(p->inputname) && p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified. When the input is a FITS " "file, a HDU must also be specified, you can use the `--hdu' " "(`-h') option and give it the HDU number (starting from " "zero), extension name, or anything acceptable by CFITSIO"); } else error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void ui_preparations(struct mknoiseparams *p) { /* Read the input image as a double type */ p->input=gal_fits_img_read_to_type(p->inputname, p->cp.hdu, GAL_TYPE_FLOAT64, p->cp.minmapsize, 0,0); /* If we are dealing with an input table, make sure the format of the output table is valid, given the type of the output. */ if(p->input->ndim==1) gal_tableintern_check_fits_format(p->cp.output, p->cp.tableformat); /* Set the output name: */ if(p->cp.output) gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); else p->cp.output=gal_checkset_automatic_output(&p->cp, p->inputname, "_noised.fits"); /* Convert the background value from magnitudes to flux. Note that magnitudes are actually calculated from the ratio of brightness, not flux. But in the context of MakeNoise where everything is done on pixels independently, brightness and flux are the same (flux is multiplied by the area of one pixel (=1) to give brightness).*/ if( !isnan(p->background_mag) ) p->background=pow(10, (p->zeropoint-p->background_mag)/2.5f); /* Allocate the random number generator: */ gsl_rng_env_setup(); p->rng=gsl_rng_alloc(gsl_rng_ranlxs1); p->rng_seed = ( p->envseed ? gsl_rng_default_seed : gal_timing_time_based_rng_seed() ); gsl_rng_set(p->rng, p->rng_seed); gal_checkset_allocate_copy(gsl_rng_name(p->rng), &p->rng_type); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct mknoiseparams *p) { struct gal_options_common_params *cp=&p->cp; char message[GAL_TIMING_VERB_MSG_LENGTH_V]; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Everything is ready, notify the user of the program starting. */ if(!p->cp.quiet) { printf(PROGRAM_NAME" started on %s", ctime(&p->rawtime)); sprintf(message, "Random number generator type: %s", gsl_rng_name(p->rng)); gal_timing_report(NULL, message, 1); sprintf(message, "Random number generator seed: %"PRId64, p->rng_seed); gal_timing_report(NULL, message, 1); } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct mknoiseparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->cp.hdu); free(p->rng_type); free(p->cp.output); gal_data_free(p->input); /* Print the final message. */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); } ��������������������gnuastro-0.5/bin/mknoise/main.c���������������������������������������������������������������������0000644�0001750�0001750�00000003167�13121462410�013447� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeNoise - Add noise to a dataset. MakeNoise is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" /* needs main.h. */ #include "mknoise.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct mknoiseparams p={{{0},0},0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ mknoise(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/Makefile.in����������������������������������������������������������������0000644�0001750�0001750�00000211331�13217217705�014431� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright 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GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME 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ps-am tags tags-am uninstall \ uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/astmknoise.conf������������������������������������������������������������0000644�0001750�0001750�00000002010�13136637645�015411� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for MakeNoise. # MakeNoise is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. 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This file is offered as-is, without any # warranty. # Input: background -10.00 instrumental 0.000 zeropoint 0.00 # Output: type float32 # Common options ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mknoise/Makefile.am����������������������������������������������������������������0000644�0001750�0001750�00000002575�13121462410�014415� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astmknoise astmknoise_LDADD = -lgnuastro astmknoise_SOURCES = main.c ui.c mknoise.c EXTRA_DIST = main.h authors-cite.h args.h ui.h mknoise.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmknoise.conf �����������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/�������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220467�012737� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/upperlimit.h�������������������������������������������������������������0000644�0001750�0001750�00000002136�13121462410�015212� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UPPERLIMIT_H #define UPPERLIMIT_H void upperlimit_calculate(struct mkcatalog_passparams *pp); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/columns.h����������������������������������������������������������������0000644�0001750�0001750�00000002207�13121462410�014477� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef COLUMNS_H #define COLUMNS_H void columns_define_alloc(struct mkcatalogparams *p); void columns_fill(struct mkcatalog_passparams *pp); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/mkcatalog.h��������������������������������������������������������������0000644�0001750�0001750�00000004435�13121462410�014766� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MKCATALOG_H #define MKCATALOG_H struct mkcatalog_passparams { struct mkcatalogparams *p; /* Main MakeCatalog paramers. */ double *oi; /* Intermediate values for objects. */ double *ci; /* Intermediate values for clumps. */ int32_t object; /* Object that is currently working on. */ size_t clumpsinobj; /* The number of clumps in this object. */ gal_data_t *tile; /* The tile to pass-over. */ float *st_i; /* Starting pointer for input image. */ int32_t *st_o; /* Starting pointer for objects image. */ int32_t *st_c; /* Starting pointer for objects image. */ float *st_sky; /* Starting pointer for input image. */ float *st_std; /* Starting pointer for input image. */ size_t start_end_inc[2]; /* Starting and ending indexs. */ size_t *shift; /* Shift coordinates for coordinates. */ gsl_rng *rng; /* Random number generator. */ size_t clumpstartindex; /* Clump starting row in final catalog. */ gal_data_t *up_vals; /* Container for upper-limit values. */ }; void mkcatalog(struct mkcatalogparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/ui.h���������������������������������������������������������������������0000644�0001750�0001750�00000006776�13216276304�013465� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_UPPERLIMIT = GAL_OPTIONS_GROUP_AFTER_COMMON, UI_GROUP_COLUMNS_IDS, UI_GROUP_COLUMNS_POSITION_PIXEL, UI_GROUP_COLUMNS_POSITION_WCS, UI_GROUP_COLUMNS_BRIGHTNESS, UI_GROUP_COLUMNS_MORPHOLOGY, }; /* Available letters for short options: f g k l u v w x y z H J L W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_OBJECTSFILE = 'O', /* General settings. */ UI_KEY_CLUMPSFILE = 'C', UI_KEY_SKYFILE = 's', UI_KEY_STDFILE = 't', UI_KEY_SKYSUBTRACTED = 'E', UI_KEY_THRESHOLD = 'R', UI_KEY_ENVSEED = 'e', UI_KEY_IDS = 'i', /* Catalog columns. */ UI_KEY_HOSTOBJID = 'j', UI_KEY_NUMCLUMPS = 'c', UI_KEY_AREA = 'a', UI_KEY_X = 'x', UI_KEY_Y = 'y', UI_KEY_RA = 'r', UI_KEY_DEC = 'd', UI_KEY_BRIGHTNESS = 'b', UI_KEY_MAGNITUDE = 'm', UI_KEY_MAGNITUDEERR = 'G', UI_KEY_UPPERLIMITMAG = 'u', UI_KEY_SN = 'n', UI_KEY_SEMIMAJOR = 'A', UI_KEY_SEMIMINOR = 'B', UI_KEY_AXISRATIO = 'Q', UI_KEY_POSITIONANGLE = 'p', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_OBJECTSHDU = 1000, /* General settings. */ UI_KEY_CLUMPSHDU, UI_KEY_SKYHDU, UI_KEY_STDHDU, UI_KEY_ZEROPOINT, UI_KEY_SFMAGNSIGMA, UI_KEY_SFMAGAREA, UI_KEY_UPMASKFILE, UI_KEY_UPMASKHDU, UI_KEY_UPNUM, UI_KEY_UPRANGE, UI_KEY_UPSIGMACLIP, UI_KEY_UPNSIGMA, UI_KEY_OBJID, /* Catalog columns. */ UI_KEY_IDINHOSTOBJ, UI_KEY_CLUMPSAREA, UI_KEY_WEIGHTAREA, UI_KEY_GEOX, UI_KEY_GEOY, UI_KEY_CLUMPSX, UI_KEY_CLUMPSY, UI_KEY_CLUMPSGEOX, UI_KEY_CLUMPSGEOY, UI_KEY_W1, UI_KEY_W2, UI_KEY_GEOW1, UI_KEY_GEOW2, UI_KEY_CLUMPSW1, UI_KEY_CLUMPSW2, UI_KEY_CLUMPSGEOW1, UI_KEY_CLUMPSGEOW2, UI_KEY_CLUMPSBRIGHTNESS, UI_KEY_NORIVERBRIGHTNESS, UI_KEY_CLUMPSMAGNITUDE, UI_KEY_UPPERLIMIT, UI_KEY_RIVERAVE, UI_KEY_RIVERNUM, UI_KEY_SKY, UI_KEY_STD, UI_KEY_GEOSEMIMAJOR, UI_KEY_GEOSEMIMINOR, UI_KEY_GEOAXISRATIO, UI_KEY_GEOPOSITIONANGLE, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct mkcatalogparams *p); void ui_free_report(struct mkcatalogparams *p, struct timeval *t1); #endif ��gnuastro-0.5/bin/mkcatalog/args.h�������������������������������������������������������������������0000644�0001750�0001750�00000054302�13216276304�013770� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { /* Input options. */ { "objectsfile", UI_KEY_OBJECTSFILE, "STR", 0, "Image containing object/detection labels.", GAL_OPTIONS_GROUP_INPUT, &p->objectsfile, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "objectshdu", UI_KEY_OBJECTSHDU, "STR", 0, "Object image extension name or number.", GAL_OPTIONS_GROUP_INPUT, &p->objectshdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "clumpsfile", UI_KEY_CLUMPSFILE, "STR", 0, "Image containing clump labels.", GAL_OPTIONS_GROUP_INPUT, &p->clumpsfile, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "clumpshdu", UI_KEY_CLUMPSHDU, "STR", 0, "Clump image extension name or number.", GAL_OPTIONS_GROUP_INPUT, &p->clumpshdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "skyfile", UI_KEY_SKYFILE, "STR", 0, "Image containing sky values.", GAL_OPTIONS_GROUP_INPUT, &p->skyfile, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "skyhdu", UI_KEY_SKYHDU, "STR", 0, "Sky image extension name or number.", GAL_OPTIONS_GROUP_INPUT, &p->skyhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "stdfile", UI_KEY_STDFILE, "STR", 0, "Image containing sky STD values.", GAL_OPTIONS_GROUP_INPUT, &p->stdfile, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "stdhdu", UI_KEY_STDHDU, "STR", 0, "Sky image extension name or number.", GAL_OPTIONS_GROUP_INPUT, &p->stdhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "zeropoint", UI_KEY_ZEROPOINT, "FLT", 0, "Zeropoint magnitude of input dataset.", GAL_OPTIONS_GROUP_INPUT, &p->zeropoint, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "skysubtracted", UI_KEY_SKYSUBTRACTED, 0, 0, "Input is already sky subtracted (for S/N).", GAL_OPTIONS_GROUP_INPUT, &p->skysubtracted, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "threshold", UI_KEY_THRESHOLD, "FLT", 0, "Use pixels more than this multiple of STD.", GAL_OPTIONS_GROUP_INPUT, &p->threshold, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Output. */ { "sfmagnsigma", UI_KEY_SFMAGNSIGMA, "FLT", 0, "Surface brightness multiple of Sky STD.", GAL_OPTIONS_GROUP_OUTPUT, &p->sfmagnsigma, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "sfmagarea", UI_KEY_SFMAGAREA, "FLT", 0, "Surface brightness area (in arcseconds^2).", GAL_OPTIONS_GROUP_OUTPUT, &p->sfmagarea, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Upper limit magnitude configurations. */ { 0, 0, 0, 0, "Upper limit magnitude settings:", UI_GROUP_UPPERLIMIT }, { "upmaskfile", UI_KEY_UPMASKFILE, "STR", 0, "Mask image file name only for upper limit.", UI_GROUP_UPPERLIMIT, &p->upmaskfile, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "upmaskhdu", UI_KEY_UPMASKHDU, "STR", 0, "Mask image HDU only for upper limit.", UI_GROUP_UPPERLIMIT, &p->upmaskhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "upnum", UI_KEY_UPNUM, "INT", 0, "Number of randomly positioned samples", UI_GROUP_UPPERLIMIT, &p->upnum, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "uprange", UI_KEY_UPRANGE, "INT,INT", 0, "Range of random positions (pix) around target.", UI_GROUP_UPPERLIMIT, &p->uprange, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_sizes_reverse }, { "envseed", UI_KEY_ENVSEED, 0, 0, "Use GSL_RNG_SEED environment variable for seed.", UI_GROUP_UPPERLIMIT, &p->envseed, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "upsigmaclip", UI_KEY_UPSIGMACLIP, "FLT,FLT", 0, "Sigma multiple and, tolerance or number.", UI_GROUP_UPPERLIMIT, &p->upsigmaclip, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_read_sigma_clip }, { "upnsigma", UI_KEY_UPNSIGMA, "FLT", 0, "Multiple of sigma to define upperlimit.", UI_GROUP_UPPERLIMIT, &p->upnsigma, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, /* ID related columns. */ { 0, 0, 0, 0, "Identifier columns", UI_GROUP_COLUMNS_IDS }, { /* `ids' is not a unique column, it is a combination of several columns. */ "ids", UI_KEY_IDS, 0, 0, "All IDs of objects and clumps.", UI_GROUP_COLUMNS_IDS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "objid", UI_KEY_OBJID, 0, 0, "Object label/ID.", UI_GROUP_COLUMNS_IDS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "hostobjid", UI_KEY_HOSTOBJID, 0, 0, "ID of object hosting this clump.", UI_GROUP_COLUMNS_IDS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "idinhostobj", UI_KEY_IDINHOSTOBJ, 0, 0, "ID of clump in host object.", UI_GROUP_COLUMNS_IDS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, /* Position related columns (pixel). */ { 0, 0, 0, 0, "Positional columns (pixel)", UI_GROUP_COLUMNS_POSITION_PIXEL }, { "x", UI_KEY_X, 0, 0, "Flux weighted center in first FITS axis.", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "y", UI_KEY_Y, 0, 0, "Flux weighted center in second FITS axis.", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geox", UI_KEY_GEOX, 0, 0, "Geometric center in first FITS axis.", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geoy", UI_KEY_GEOY, 0, 0, "Geometric center in second FITS axis.", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsx", UI_KEY_CLUMPSX, 0, 0, "Flux.wht center of all clumps in obj. (X).", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsy", UI_KEY_CLUMPSY, 0, 0, "Flux.wht center of all clumps in obj. (Y).", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsgeox", UI_KEY_CLUMPSGEOX, 0, 0, "Geometric center of all clumps in obj. (X).", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsgeoy", UI_KEY_CLUMPSGEOY, 0, 0, "Geometric center of all clumps in obj. (Y).", UI_GROUP_COLUMNS_POSITION_PIXEL, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, /* Position related columns (WCS). */ { 0, 0, 0, 0, "Positional columns (WCS)", UI_GROUP_COLUMNS_POSITION_WCS }, { "ra", UI_KEY_RA, 0, 0, "Flux weighted center right ascension.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "dec", UI_KEY_DEC, 0, 0, "Flux weighted center declination.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "w1", UI_KEY_W1, 0, 0, "Flux weighted center in first WCS axis.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "w2", UI_KEY_W2, 0, 0, "Flux weighted center in second WCS axis.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geow1", UI_KEY_GEOW1, 0, 0, "Geometric center in first WCS axis.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geow2", UI_KEY_GEOW2, 0, 0, "Geometric center in second WCS axis.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsw1", UI_KEY_CLUMPSW1, 0, 0, "Flux.wht center of all clumps in 1st WCS.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsw2", UI_KEY_CLUMPSW2, 0, 0, "Flux.wht center of all clumps in 2nd WCS.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsgeow1", UI_KEY_CLUMPSGEOW1, 0, 0, "Geometric center of all clumps in 1st WCS.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsgeow2", UI_KEY_CLUMPSGEOW2, 0, 0, "Geometric center of all clumps in 2nd WCS.", UI_GROUP_COLUMNS_POSITION_WCS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, /* Brightness/pixel-value related columns. */ { 0, 0, 0, 0, "Brightness/magnitude related columns", UI_GROUP_COLUMNS_BRIGHTNESS }, { "brightness", UI_KEY_BRIGHTNESS, 0, 0, "Brightness (sum of pixel values).", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpbrightness", UI_KEY_CLUMPSBRIGHTNESS, 0, 0, "Brightness of clumps in an object.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "noriverbrightness", UI_KEY_NORIVERBRIGHTNESS, 0, 0, "Sky (not river) subtracted clump brightness.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "magnitude", UI_KEY_MAGNITUDE, 0, 0, "Total magnitude of objects or clumps.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "magnitudeerr", UI_KEY_MAGNITUDEERR, 0, 0, "Magnitude error of objects or clumps.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsmagnitude", UI_KEY_CLUMPSMAGNITUDE, 0, 0, "Magnitude of all clumps in object.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "upperlimit", UI_KEY_UPPERLIMIT, 0, 0, "Upper-limit value, use other options to config.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "upperlimitmag", UI_KEY_UPPERLIMITMAG, 0, 0, "Upper-limit mag. use other options to config.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "riverave", UI_KEY_RIVERAVE, 0, 0, "Average river value surrounding a clump.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "rivernum", UI_KEY_RIVERNUM, 0, 0, "Number of river pixels around a clump.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "sn", UI_KEY_SN, 0, 0, "Signal to noise ratio of objects or clumps.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "sky", UI_KEY_SKY, 0, 0, "Average Sky value under this clump or object.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "std", UI_KEY_STD, 0, 0, "Average Sky standard deviation.", UI_GROUP_COLUMNS_BRIGHTNESS, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, /* Morphology/shapre related columns. */ { 0, 0, 0, 0, "Morphology/shape related columns", UI_GROUP_COLUMNS_MORPHOLOGY }, { "numclumps", UI_KEY_NUMCLUMPS, 0, 0, "Number of clumps in this object.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "area", UI_KEY_AREA, 0, 0, "Number of pixels in clump or object.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "clumpsarea", UI_KEY_CLUMPSAREA, 0, 0, "Sum of all clump areas in an object.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "weightarea", UI_KEY_WEIGHTAREA, 0, 0, "Area used for flux weighted positions.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "semimajor", UI_KEY_SEMIMAJOR, 0, 0, "Flux weighted semi-major axis.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "semiminor", UI_KEY_SEMIMINOR, 0, 0, "Flux weighted semi-minor axis.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "axisratio", UI_KEY_AXISRATIO, 0, 0, "Flux weighted axis ratio.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "positionangle", UI_KEY_POSITIONANGLE, 0, 0, "Flux weighted position angle.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geosemimajor", UI_KEY_GEOSEMIMAJOR, 0, 0, "Geometric semi-major axis.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geosemiminor", UI_KEY_GEOSEMIMINOR, 0, 0, "Geometric semi-minor axis.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geoaxisratio", UI_KEY_GEOAXISRATIO, 0, 0, "Geometric axis ratio.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, { "geopositionangle", UI_KEY_GEOPOSITIONANGLE, 0, 0, "Geometric position angle.", UI_GROUP_COLUMNS_MORPHOLOGY, 0, GAL_TYPE_INVALID, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_column_codes_ll }, {0} }; /* Define the child argp structure ------------------------------- NOTE: these parts can be left untouched.*/ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/authors-cite.h�����������������������������������������������������������0000644�0001750�0001750�00000005205�13211076737�015444� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX \ "Description of MakeCatalog\n" \ "--------------------------\n" \ "@ARTICLE{2016arXiv161106387A,\n" \ " author = {{Akhlaghi}, M.},\n" \ " title = \"{Separating detection and catalog production}\",\n" \ " journal = {ASP Conf. Ser. (in press)},\n" \ "archivePrefix = \"arXiv\",\n" \ " eprint = {1611.06387},\n" \ "primaryClass = \"astro-ph.IM\",\n" \ " keywords = {Astrophysics - Instrumentation and Methods for " \ "Astrophysics},\n" \ " year = 2016,\n" \ " month = nov,\n" \ " adsurl = {http://adsabs.harvard.edu/abs/2016arXiv161106387A},\n" \ " adsnote = {Provided by the SAO/NASA Astrophysics Data System}\n" \ "};\n" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/main.h�������������������������������������������������������������������0000644�0001750�0001750�00000026042�13216276304�013760� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gsl/gsl_rng.h> #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "MakeCatalog" /* Program full name. */ #define PROGRAM_EXEC "astmkcatalog" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Multiple of given number to stop searching for upper-limit magnitude. */ #define MKCATALOG_UPPERLIMIT_STOP_MULTIP 50 #define MKCATALOG_UPPERLIMIT_MINIMUM_NUM 20 /* Intermediate/raw array elements =============================== Commonly, several high-level calculations need the same low-level measurements. So to avoid having to do these low-level calculations on each pixel multiple tiles, each thread/object will have one array of intermediate values which will be filled in the pass over the pixels. After this intermediate array is filled, and we don't need to pass over the pixels any more, we will use the intermediate values to derive the higher-level steps. According to the C standard, the first enum variable has a value of 0 (int), and when none are explicitly set (with an = sign), the values of the subsequent enum variables are 1 larger. We want column indexs that also start with zero, but setting the values by hand manually as preprocessor macros can be buggy (repeated numbers). So defining them as an enum is the perfect solution. Any future column that is to be added (or if any are removed), we (the developers) don't have to worry. --------------------- POSITIONS IN FITS standard --------------------- Like the final output, positions in this intermediate array are also in the FITS standard (fastest dimension is first). */ enum objectcols { OCOL_NUMALL, /* Number of all pixels with this label. */ OCOL_NUM, /* Number of pixels above threshold. */ OCOL_SUM, /* Sum of (value-sky) in object. */ OCOL_VX, /* Sum of (value-sky) * x. */ OCOL_VY, /* Sum of (value-sky) * y. */ OCOL_SX, /* Shift along X axis. */ OCOL_SY, /* Shift along Y axis. */ OCOL_VXX, /* Sum of (value-sky) * x * x. */ OCOL_VYY, /* Sum of (value-sky) * y * y. */ OCOL_VXY, /* Sum of (value-sky) * x * y. */ OCOL_SUMSKY, /* Sum of sky value on this object. */ OCOL_SUMSTD, /* Sum of sky STD value on this object. */ OCOL_SUMWHT, /* Sum of positive image pixels. */ OCOL_NUMWHT, /* Number of positive pixels used for wht. */ OCOL_GX, /* Geometric center of object in X. */ OCOL_GY, /* Geometric center of object in Y. */ OCOL_GXX, /* Second order geometric variable: X*X. */ OCOL_GYY, /* Second order geometric variable: Y*Y. */ OCOL_GXY, /* Second order geometric variable: X*Y. */ OCOL_UPPERLIMIT_B, /* Upper limit magnitude. */ OCOL_C_NUMALL, /* Value independent no. of pixels in clumps.*/ OCOL_C_NUM, /* Area of clumps in this object. */ OCOL_C_SUM, /* Brightness in object clumps. */ OCOL_C_VX, /* Sum of (value-sky)*x on clumps. */ OCOL_C_VY, /* Sum of (value-sky)*y on obj. clumps. */ OCOL_C_GX, /* Geometric center of clumps in object X. */ OCOL_C_GY, /* Geometric center of clumps in object Y. */ OCOL_C_SUMWHT, /* Sum of positive image pixels for wht. */ OCOL_C_NUMWHT, /* Num of positive image pixels for wht. */ OCOL_NUMCOLS, /* SHOULD BE LAST: total number of columns. */ }; enum clumpcols { CCOL_NUMALL, /* Area of clump irrespective of threshold. */ CCOL_NUM, /* Area of this clump. */ CCOL_VX, /* Sum of (value-sky) * x. */ CCOL_VY, /* Sum of (value-sky) * y. */ CCOL_VXX, /* Sum of flux*x*x of this clump. */ CCOL_VYY, /* Sum of flux*y*y of this clump. */ CCOL_VXY, /* Sum of flux*x*y of this clump. */ CCOL_SUM, /* River subtracted brightness. */ CCOL_RIV_SUM, /* Sum of rivers around clump. */ CCOL_RIV_NUM, /* Num river pixels around this clump. */ CCOL_SUMSKY, /* Sum of sky value on this object. */ CCOL_SUMSTD, /* Sum of sky STD value on this object. */ CCOL_SUMWHT, /* Sum of positive image pixels for wht. */ CCOL_NUMWHT, /* Num of positive image pixels for wht. */ CCOL_GX, /* Geometric center of clump in X. */ CCOL_GY, /* Geometric center of clump in Y. */ CCOL_GXX, /* Second order geometric moment. */ CCOL_GYY, /* Second order geometric moment. */ CCOL_GXY, /* Second order geometric moment. */ CCOL_UPPERLIMIT_B, /* Upper limit magnitude. */ CCOL_NUMCOLS, /* SHOULD BE LAST: total number of columns. */ }; /* Main program parameters structure */ struct mkcatalogparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ gal_list_i32_t *columnids; /* The desired column codes. */ char *inputname; /* Input filename. */ char *objectsfile; /* File name of objects file. */ char *objectshdu; /* HDU of objects image. */ char *clumpsfile; /* File name of objects file. */ char *clumpshdu; /* HDU of objects image. */ char *skyfile; /* File name of sky file. */ char *skyhdu; /* HDU of sky image. */ char *stdfile; /* File name of sky STD file. */ char *stdhdu; /* HDU of sky STD image. */ float zeropoint; /* Zero-point magnitude of object. */ uint8_t skysubtracted; /* If image is already sky subtracted. */ float threshold; /* Only use values above this threshold.*/ float sfmagnsigma; /* Surface brightness multiple of sigma.*/ float sfmagarea; /* Surface brightness area (arcsec^2). */ char *upmaskfile; /* Name of upper limit mask file. */ char *upmaskhdu; /* HDU of upper limit mask file. */ size_t upnum; /* Number of upper-limit random samples.*/ size_t *uprange; /* Range of random positions about target. */ uint8_t envseed; /* Use the environment for random seed. */ double upsigmaclip[2]; /* Sigma clip to measure upper limit. */ float upnsigma; /* Multiple of sigma to define up-lim. */ /* Internal. */ time_t rawtime; /* Starting time of the program. */ gal_data_t *input; /* Input. */ gal_data_t *objects; /* Object labels. */ gal_data_t *clumps; /* Clump labels. */ gal_data_t *sky; /* Sky. */ gal_data_t *std; /* Sky standard deviation. */ gal_data_t *upmask; /* Upper limit magnitude mask. */ float minstd; /* Minimum Standard deviation value. */ float medstd; /* Median standard deviation value. */ float cpscorr; /* Counts-per-second correction. */ float detsn; /* Minimum detection S/N threshold. */ size_t numobjects; /* Number of object labels in image. */ float clumpsn; /* Clump S/N threshold. */ size_t numclumps; /* Number of clumps in image. */ gal_data_t *objectcols; /* Output columns for the objects. */ gal_data_t *clumpcols; /* Output columns for the clumps. */ gal_data_t *tiles; /* Tiles to cover each object. */ char *objectsout; /* Output objects catalog. */ char *clumpsout; /* Output clumps catalog. */ uint8_t *oiflag; /* Intermediate flags for objects. */ uint8_t *ciflag; /* Intermediate flags for clumps. */ pthread_mutex_t mutex; /* Mutex to change the total numbers. */ size_t clumprowsfilled; /* No. filled clump rows at this moment.*/ gsl_rng *rng; /* Main random number generator. */ uint64_t seed; /* Random number generator seed. */ const char *rngname; /* Name of random number generator. */ size_t rngmin; /* Minimum possible value of RNG. */ size_t rngdiff; /* Difference of RNG max and min. */ gal_data_t *wcs_vo; /* Object RA-Dec flux weighted X, Y. */ gal_data_t *wcs_vc; /* Clump RA-Dec flux weighted X, Y. */ gal_data_t *wcs_go; /* Object RA-Dec geometric X,Y. */ gal_data_t *wcs_gc; /* Clump RA-Dec geometric X, Y. */ gal_data_t *wcs_vcc; /* All clumps RA-Dec flx. wht. X, Y. */ gal_data_t *wcs_gcc; /* All clumps RA-Dec geometric X, Y. */ char **ctype; /* Type of WCS axis. */ uint8_t hasblank; /* Dataset has blank values. */ uint8_t hasmag; /* Catalog has magnitude columns. */ uint8_t upperlimit; /* Calculate upper limit magnitude. */ }; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/upperlimit.c�������������������������������������������������������������0000644�0001750�0001750�00000035113�13216276304�015220� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <float.h> #include <stdlib.h> #include <gnuastro/tile.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro/statistics.h> #include "main.h" #include "mkcatalog.h" /*********************************************************************/ /******************* Tiles for clumps ********************/ /*********************************************************************/ static gal_data_t * upperlimit_make_clump_tiles(struct mkcatalog_passparams *pp) { gal_data_t *input=pp->p->input; size_t ndim=input->ndim, *dsize=input->dsize; int32_t *O, *C; gal_data_t *tiles=NULL; float *I, *II, *start=input->array; size_t increment=0, num_increment=1; size_t i, d, *min, *max, width=2*ndim; size_t *coord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "coord"); size_t *minmax=gal_data_malloc_array(GAL_TYPE_SIZE_T, width*pp->clumpsinobj, __func__, "minmax"); /* Initialize the minimum and maximum position for each tile/clump. So, we'll initialize the minimum coordinates to the maximum possible `size_t' value (in `GAL_BLANK_SIZE_T') and the maximums to zero. */ for(i=0;i<pp->clumpsinobj;++i) for(d=0;d<ndim;++d) { minmax[ i * width + d ] = GAL_BLANK_SIZE_T; /* Minimum. */ minmax[ i * width + ndim + d ] = 0; /* Maximum. */ } /* Parse over the object and get the clump's minimum and maximum. */ while( pp->start_end_inc[0] + increment <= pp->start_end_inc[1] ) { /* Set the pointers for this tile. */ I = pp->st_i + increment; O = pp->st_o + increment; C = pp->st_c + increment; /* Go over the contiguous region. */ II = I + dsize[ndim-1]; do { /* Only consider clumps. */ if( *O==pp->object && *C>0 ) { /* Get the coordinates of this pixel. */ gal_dimension_index_to_coord(I-start, ndim, dsize, coord); /* Check to see if this coordinate is the smallest/largest found so far for this label. Note that labels start from 1, while indexs here start from zero. */ min = &minmax[ (*C-1) * width ]; max = &minmax[ (*C-1) * width + ndim ]; for(d=0;d<ndim;++d) { if( coord[d] < min[d] ) min[d] = coord[d]; if( coord[d] > max[d] ) max[d] = coord[d]; } } /* Increment the other pointers. */ ++O; ++C; } while(++I<II); /* Increment to the next contiguous region. */ increment += ( gal_tile_block_increment(input, dsize, num_increment++, NULL) ); } /* For a check. for(i=0;i<pp->clumpsinobj;++i) printf("%zu: (%zu, %zu) --> (%zu, %zu)\n", i+1, minmax[i*width], minmax[i*width+1], minmax[i*width+2], minmax[i*width+3]); */ /* Make the tiles. */ tiles=gal_tile_series_from_minmax(input, minmax, pp->clumpsinobj); /* Cleanup and return. */ free(coord); free(minmax); return tiles; } /*********************************************************************/ /******************* For one tile ********************/ /*********************************************************************/ static void upperlimit_random_range(struct mkcatalog_passparams *pp, gal_data_t *tile, size_t *min, size_t *max, int32_t clumplab) { struct mkcatalogparams *p=pp->p; size_t d, tstart, minext, maxext, coord[]={0,0}; size_t ndim=p->input->ndim, *dsize=p->input->dsize; /* Set the minimum and maximum acceptable value for the range. */ if(p->uprange) { tstart=gal_data_ptr_dist(tile->block->array, tile->array, p->input->type); gal_dimension_index_to_coord(tstart, ndim, dsize, coord); } /* Go over the dimensions and set the range along each dimension. */ for(d=0;d<ndim;++d) { /* If uprange is given and it is not zero, then use it, otherwise, just use the full possible range. */ if( p->uprange && p->uprange[d] ) { /* Set the minimum of the random range. Since `size_t' is always positive, to make sure the difference isn't negative, we need to convert them to integer first. */ if( (int)coord[d] - ((int)p->uprange[d])/2 > 0 ) { min[d] = coord[d]-p->uprange[d]/2; maxext = 0; } else { min[d] = 0; maxext = -1 * ((int)coord[d] - ((int)p->uprange[d])/2); } /* Set the maximum of the random range. */ if( coord[d] + p->uprange[d]/2 < dsize[d] - tile->dsize[d] ) { max[d] = coord[d] + p->uprange[d]/2; minext = 0; } else { max[d] = dsize[d] - tile->dsize[d] - 1; minext = ( (coord[d] + p->uprange[d]/2) - (dsize[d] - tile->dsize[d]) ); } /* `minadd' and `maxadd' were defined to account for the removed smaller range when an object is on the edge. Their role is to add to the other side of the range as much as possible when one side is decreased on an edge. */ if(minext) min[d] = ((int)(min[d]) - (int)minext >= 0) ? (min[d]-minext) : 0; if(maxext) max[d] = ( (max[d] + maxext < dsize[d] - tile->dsize[d]) ? (max[d] + maxext) : (dsize[d]-tile->dsize[d]-1) ); } else { min[d]=0; max[d]=dsize[d]-tile->dsize[d]-1; } /* A small sanity check. */ if( max[d]-min[d] < 2*tile->dsize[d] ) { if(clumplab) fprintf(stderr, "WARNING: object %d clump %d: range of random " "positions (%zu) along dimension %zu for upper-limit " "calculations is smaller than double of its size (%zu) " "in this dimension.\n\n", pp->object, clumplab, max[d]-min[d], ndim-d, 2*tile->dsize[d]); else fprintf(stderr, "WARNING: object %d: range of random " "positions (%zu) along dimension %zu for upper-limit " "calculations is smaller than double of its size (%zu) " "in this dimension.\n\n", pp->object, max[d]-min[d], ndim-d, 2*tile->dsize[d]); } } } /* Return a random position in the requested dimension. */ static size_t upperlimit_random_position(struct mkcatalog_passparams *pp, gal_data_t *tile, size_t dim, size_t *min, size_t *max) { size_t r; struct mkcatalogparams *p=pp->p; /* `gsl_rng_get' returns an inclusive value between the minimum and maximum of the particular generator. It may happen that the labeled region extends the full range of a dimension. In that case, the only possible starting point would be 0. */ if( (int)(p->input->dsize[dim]) - (int)(tile->dsize[dim]) > 0 ) { r=gsl_rng_get(pp->rng); /* For easy reading. */ return lrint( (float)(min[dim]) + ( (float)(r-p->rngmin)/(float)(p->rngdiff) * (float)(max[dim] - min[dim]) ) ); } else return 0; } static double upperlimit_one_tile(struct mkcatalog_passparams *pp, gal_data_t *tile, unsigned long seed, int32_t clumplab) { struct mkcatalogparams *p=pp->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; void *tarray; double sum, out; int continueparse; gal_data_t *sigclip; uint8_t *M=NULL, *st_m=NULL; float *uparr=pp->up_vals->array; float *I, *II, *SK, *st_i, *st_sky; size_t d, tcounter=0, counter=0, se_inc[2]; size_t min[2], max[2], increment, num_increment; int32_t *O, *oO, *st_o, *st_oo, *st_oc, *oC=NULL; size_t maxcount = p->upnum * MKCATALOG_UPPERLIMIT_STOP_MULTIP; size_t *rcoord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "rcoord"); /* Initializations. */ tarray=tile->array; gsl_rng_set(pp->rng, seed); /* Set the range of random values for this tile. */ upperlimit_random_range(pp, tile, min, max, clumplab); /* `se_inc' is just used temporarily, the important thing here is `st_oo'. */ st_oo = ( clumplab ? gal_tile_start_end_ind_inclusive(tile, p->objects, se_inc) : pp->st_o ); st_oc = clumplab ? (int32_t *)(p->clumps->array) + se_inc[0] : NULL; /* Continue measuring randomly until we get the desired total number. */ while(tcounter<maxcount && counter<p->upnum) { /* Get the random coordinates. */ for(d=0;d<ndim;++d) rcoord[d] = upperlimit_random_position(pp, tile, d, min, max); /* Set the tile's new starting pointer. */ tile->array = gal_data_ptr_increment(p->input->array, gal_dimension_coord_to_index(ndim, dsize, rcoord), p->input->type); /* Starting and ending coordinates for this random position, note that in `pp' we have the starting and ending coordinates of the actual tile. */ increment = 0; num_increment = 1; continueparse = 1; sum = 0.0f; /* Starting pointers for the random tile. */ st_i = gal_tile_start_end_ind_inclusive(tile, p->input, se_inc); st_o = (int32_t *)(p->objects->array) + se_inc[0]; st_sky = (float *)(p->sky->array) + se_inc[0]; if(p->upmask) st_m = (uint8_t *)(p->upmask->array) + se_inc[0]; /* Parse over this object/clump. */ while( se_inc[0] + increment <= se_inc[1] ) { /* Set the pointers. */ I = st_i + increment; /* Random tile. */ SK = st_sky + increment; /* Random tile. */ O = st_o + increment; /* Random tile. */ if(st_m) M = st_m + increment; /* Random tile. */ oO = st_oo + increment; /* Original tile. */ if(clumplab) oC = st_oc + increment; /* Original tile. */ /* Parse over this contiguous region, similar to the first and second pass functions. */ II = I + tile->dsize[ndim-1]; do { /* Only use pixels over this object/clump. */ if( *oO==pp->object && ( oC==NULL || clumplab==0 || *oC==clumplab ) ) { if( *O || (M && *M) || ( p->hasblank && isnan(*I) ) ) continueparse=0; else sum += *I-*SK; } /* Increment the other pointers. */ ++SK; ++O; ++oO; if(oC) ++oC; } while(continueparse && ++I<II); /* Increment to the next contiguous region of this tile. */ if(continueparse) increment += ( gal_tile_block_increment(p->input, dsize, num_increment++, NULL) ); else break; } /* Further processing is only necessary if this random tile actually covered the sky region. */ if(continueparse) uparr[ counter++ ] = sum; /* Increment the total-counter. */ ++tcounter; } /* Calculate the standard deviation of this distribution. */ if(counter==p->upnum) { sigclip=gal_statistics_sigma_clip(pp->up_vals, p->upsigmaclip[0], p->upsigmaclip[1], 1, 1); out = ((float *)(sigclip->array))[3] * p->upnsigma; } else out=NAN; /* Reset the tile's array pointer, clean up and return. */ tile->array=tarray; free(rcoord); return out; } /*********************************************************************/ /******************* High level funciton ********************/ /*********************************************************************/ void upperlimit_calculate(struct mkcatalog_passparams *pp) { size_t i; double *ci; unsigned long seed; gal_data_t *clumptiles; struct mkcatalogparams *p=pp->p; /* First find the upper limit magnitude for this object. */ pp->oi[OCOL_UPPERLIMIT_B] = upperlimit_one_tile(pp, pp->tile, p->seed+pp->object, 0); /* If a clumps image is present (a clump catalog is requested( and this object has clumps, then find the upper limit magnitude for the clumps within this object. */ if(p->clumps && pp->clumpsinobj) { /* Make tiles covering the clumps. */ clumptiles=upperlimit_make_clump_tiles(pp); /* Go over all the clumps. The random number generator seed for each clump/object has to be unique, but also reproducible (given the intial seed and identical inputs). So we have defined it based on the total number of objects and clumps and this object and clump's IDs. */ for(i=0;i<pp->clumpsinobj;++i) { ci=&pp->ci[ i * CCOL_NUMCOLS ]; seed = p->seed + p->numobjects + p->numclumps * pp->object + i; ci[CCOL_UPPERLIMIT_B] = upperlimit_one_tile(pp, &clumptiles[i], seed, i+1); } /* Clean up the clump tiles. */ gal_data_array_free(clumptiles, pp->clumpsinobj, 0); } } �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/columns.c����������������������������������������������������������������0000644�0001750�0001750�00000153301�13216276304�014506� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <pthread.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "mkcatalog.h" #include "ui.h" #include "columns.h" /******************************************************************/ /******************* Intermediate arrays ******************/ /******************************************************************/ /* Allocate RA-DEC internal arrays. These arrays are defined to keep all the positions in one place and do the RA-DEC conversion once in the end. They are all allocated together, but we don't know if RA is requested first or Dec or if they are requested multiple times. So before the allocation, we'll check the first one. The space that is allocated in `columns_define_alloc' is for the final values that are written in the output file. */ static void columns_alloc_radec(struct mkcatalogparams *p) { size_t i; /* For objects. */ if(p->wcs_vo==NULL) for(i=0;i<p->input->ndim;++i) gal_list_data_add_alloc(&p->wcs_vo, NULL, GAL_TYPE_FLOAT64, 1, &p->numobjects, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* For clumps */ if(p->clumps && p->wcs_vc==NULL) for(i=0;i<p->input->ndim;++i) gal_list_data_add_alloc(&p->wcs_vc, NULL, GAL_TYPE_FLOAT64, 1, &p->numclumps, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); } /* Similar to `columns_alloc_radec'. */ static void columns_alloc_georadec(struct mkcatalogparams *p) { size_t i; /* For objects. */ if(p->wcs_go==NULL) for(i=0;i<p->input->ndim;++i) gal_list_data_add_alloc(&p->wcs_go, NULL, GAL_TYPE_FLOAT64, 1, &p->numobjects, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); /* For clumps */ if(p->clumps && p->wcs_gc==NULL) for(i=0;i<p->input->ndim;++i) gal_list_data_add_alloc(&p->wcs_gc, NULL, GAL_TYPE_FLOAT64, 1, &p->numclumps, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); } /* Similar to `columns_alloc_radec'. */ static void columns_alloc_clumpsradec(struct mkcatalogparams *p) { size_t i; if(p->wcs_vcc==NULL) for(i=0;i<p->input->ndim;++i) gal_list_data_add_alloc(&p->wcs_vcc, NULL, GAL_TYPE_FLOAT64, 1, &p->numobjects, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); } /* Similar to `columns_alloc_radec'. */ static void columns_alloc_clumpsgeoradec(struct mkcatalogparams *p) { size_t i; if(p->wcs_gcc==NULL) for(i=0;i<p->input->ndim;++i) gal_list_data_add_alloc(&p->wcs_gcc, NULL, GAL_TYPE_FLOAT64, 1, &p->numobjects, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); } /* Set pointers to fascilitate filling in the values. */ #define SET_WCS_PREPARE(ARR, LIST, ARRNAME) { \ d=0; \ errno=0; \ (ARR)=malloc(p->input->ndim * sizeof (ARR) ); \ if( (ARR)==NULL ) \ error(EXIT_FAILURE, 0, "%s: %zu bytes for %s", __func__, \ p->input->ndim * sizeof (ARR), ARRNAME); \ for(tmp=(LIST);tmp!=NULL;tmp=tmp->next) (ARR)[d++]=tmp->array; \ } static void columns_set_wcs_pointers(struct mkcatalogparams *p, double ***vo, double ***vc, double ***go, double ***gc, double ***vcc, double ***gcc) { size_t d; gal_data_t *tmp; if(p->wcs_vo) SET_WCS_PREPARE(*vo, p->wcs_vo, "vo" ); if(p->wcs_vc) SET_WCS_PREPARE(*vc, p->wcs_vc, "vc" ); if(p->wcs_go) SET_WCS_PREPARE(*go, p->wcs_go, "go" ); if(p->wcs_gc) SET_WCS_PREPARE(*gc, p->wcs_gc, "gc" ); if(p->wcs_vcc) SET_WCS_PREPARE(*vcc, p->wcs_vcc, "vcc"); if(p->wcs_gcc) SET_WCS_PREPARE(*gcc, p->wcs_gcc, "gcc"); } /******************************************************************/ /********** Column definition/allocation ***************/ /******************************************************************/ static void columns_wcs_preparation(struct mkcatalogparams *p) { size_t i; gal_list_i32_t *colcode; int continue_wcs_check=1; /* Make sure a WCS structure is present if we need it. */ for(colcode=p->columnids; colcode!=NULL; colcode=colcode->next) { if(continue_wcs_check) { switch(colcode->v) { /* High-level. */ case UI_KEY_RA: case UI_KEY_DEC: /* Low-level. */ case UI_KEY_W1: case UI_KEY_W2: case UI_KEY_GEOW1: case UI_KEY_GEOW2: case UI_KEY_CLUMPSW1: case UI_KEY_CLUMPSW2: case UI_KEY_CLUMPSGEOW1: case UI_KEY_CLUMPSGEOW2: if(p->input->wcs) continue_wcs_check=0; else error(EXIT_FAILURE, 0, "input doesn't have WCS meta-data for " "defining world coordinates (like RA and Dec). Atleast " "one of the requested columns requires this " "information"); break; } } else break; } /* Convert the high-level WCS columns to low-level ones. */ for(colcode=p->columnids; colcode!=NULL; colcode=colcode->next) switch(colcode->v) { case UI_KEY_RA: case UI_KEY_DEC: /* Check all the CTYPES. */ for(i=0;i<p->input->ndim;++i) if( !strcmp(p->ctype[i], colcode->v==UI_KEY_RA ? "RA" : "DEC") ) { colcode->v = i==0 ? UI_KEY_W1 : UI_KEY_W2; break; } /* Make sure it actually existed. */ if(i==p->input->ndim) error(EXIT_FAILURE, 0, "%s (hdu: %s): %s not present in any of " "the WCS axis types (CTYPE)", p->inputname, p->cp.hdu, colcode->v==UI_KEY_RA ? "RA" : "DEC"); break; } } /* Set the necessary parameters for each output column and allocate the space necessary to keep the values. */ void columns_define_alloc(struct mkcatalogparams *p) { gal_list_i32_t *colcode; gal_list_str_t *strtmp, *noclumpimg=NULL; int disp_fmt=0, disp_width=0, disp_precision=0; char *name=NULL, *unit=NULL, *ocomment=NULL, *ccomment=NULL; uint8_t otype=GAL_TYPE_INVALID, ctype=GAL_TYPE_INVALID, *oiflag, *ciflag; /* If there is any columns that need WCS, the input image needs to have a WCS in its headers. So before anything, we need to check if a WCS is present or not. This can't be done after the initial setting of column properties because the WCS-related columns use information that is based on it (for units and names). */ columns_wcs_preparation(p); /* Allocate the array for which intermediate parameters are necessary. The basic issue is that higher-level calculations require a smaller domain of raw measurements. So to avoid having to calculate something multiple times, each parameter will flag the intermediate parameters it requires in these arrays. */ oiflag = p->oiflag = gal_data_malloc_array(GAL_TYPE_UINT8, OCOL_NUMCOLS, __func__, "oiflag"); ciflag = p->ciflag = gal_data_malloc_array(GAL_TYPE_UINT8, CCOL_NUMCOLS, __func__, "ciflag"); /* Allocate the columns. */ for(colcode=p->columnids; colcode!=NULL; colcode=colcode->next) { /* Set the column-specific parameters, please follow the same order as `args.h'. IMPORTANT: we want the names to be the same as the option names. Note that zero `disp_' variables will be automatically determined.*/ switch(colcode->v) { case UI_KEY_OBJID: name = "OBJ_ID"; unit = "counter"; ocomment = "Object identifier."; ccomment = NULL; otype = GAL_TYPE_INT32; /* Same type as clumps image. */ ctype = GAL_TYPE_INVALID; disp_fmt = 0; disp_width = 6; disp_precision = 0; /* Is an internal parameter. */ break; case UI_KEY_HOSTOBJID: name = "HOST_OBJ_ID"; unit = "counter"; ocomment = NULL; ccomment = "Object identifier hosting this clump."; otype = GAL_TYPE_INVALID; ctype = GAL_TYPE_INT32; disp_fmt = 0; disp_width = 6; disp_precision = 0; /* Is an internal parameter. */ break; case UI_KEY_IDINHOSTOBJ: name = "ID_IN_HOST_OBJ"; unit = "counter"; ocomment = NULL; ccomment = "ID of clump in its host object."; otype = GAL_TYPE_INVALID; ctype = GAL_TYPE_INT32; disp_fmt = 0; disp_width = 6; disp_precision = 0; /* Is an internal parameter. */ break; case UI_KEY_NUMCLUMPS: name = "NUM_CLUMPS"; unit = "counter"; ocomment = "Number of clumps in this object."; ccomment = NULL; otype = GAL_TYPE_INT32; ctype = GAL_TYPE_INVALID; disp_fmt = 0; disp_width = 5; disp_precision = 0; /* Is an internal parameter. */ break; case UI_KEY_AREA: name = "AREA"; unit = "counter"; ocomment = "Number of pixels covered."; ccomment = ocomment; otype = GAL_TYPE_INT32; ctype = GAL_TYPE_INT32; disp_fmt = 0; disp_width = 5; disp_precision = 0; oiflag[ OCOL_NUMALL ] = 1; ciflag[ CCOL_NUMALL ] = 1; break; case UI_KEY_CLUMPSAREA: name = "CLUMPS_AREA"; unit = "counter"; ocomment = "Total number of clump pixels in object."; ccomment = NULL; otype = GAL_TYPE_INT32; ctype = GAL_TYPE_INVALID; disp_fmt = 0; disp_width = 5; disp_precision = 0; oiflag[ OCOL_C_NUM ] = 1; break; case UI_KEY_WEIGHTAREA: name = "WEIGHT_AREA"; unit = "counter"; ocomment = "Area used for flux-weighted positions."; ccomment = ocomment; otype = GAL_TYPE_INT32; ctype = GAL_TYPE_INT32; disp_fmt = 0; disp_width = 5; disp_precision = 0; oiflag[ OCOL_NUMWHT ] = 1; ciflag[ CCOL_NUMWHT ] = 1; break; case UI_KEY_X: name = "X"; unit = "pixel"; ocomment = "Flux weighted center (FITS axis 1)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_VX ] = 1; ciflag[ CCOL_VX ] = 1; break; case UI_KEY_Y: name = "Y"; unit = "pixel"; ocomment = "Flux weighted center (FITS axis 2)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_VY ] = 1; ciflag[ CCOL_VY ] = 1; break; case UI_KEY_GEOX: name = "GEO_X"; unit = "pixel"; ocomment = "Geometric center (FITS axis 1)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_GX ] = 1; ciflag[ CCOL_GX ] = 1; break; case UI_KEY_GEOY: name = "GEO_Y"; unit = "pixel"; ocomment = "Geometric center (FITS axis 2)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_GY ] = 1; ciflag[ CCOL_GY ] = 1; break; case UI_KEY_CLUMPSX: name = "CLUMPS_X"; unit = "pixel"; ocomment = "Flux weighted center of clumps (FITS axis 1)."; ccomment = NULL; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_C_VX ] = 1; break; case UI_KEY_CLUMPSY: name = "CLUMPS_Y"; unit = "pixel"; ocomment = "Flux weighted center of clumps (FITS axis 2)."; ccomment = NULL; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_C_VY ] = 1; break; case UI_KEY_CLUMPSGEOX: name = "CLUMPS_GEO_X"; unit = "pixel"; ocomment = "Geometric center of clumps (FITS axis 1)."; ccomment = NULL; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_C_GX ] = 1; break; case UI_KEY_CLUMPSGEOY: name = "CLUMPS_GEO_Y"; unit = "pixel"; ocomment = "Geometric center of clumps (FITS axis 2)."; ccomment = NULL; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_C_GY ] = 1; break; case UI_KEY_W1: name = p->ctype[0]; unit = p->input->wcs->cunit[0]; ocomment = "Flux weighted center (WCS axis 1)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_FLOAT64; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_VX ] = 1; oiflag[ OCOL_VY ] = 1; oiflag[ CCOL_VX ] = 1; oiflag[ CCOL_VY ] = 1; columns_alloc_radec(p); break; case UI_KEY_W2: name = p->ctype[1]; unit = p->input->wcs->cunit[1]; ocomment = "Flux weighted center (WCS axis 2)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_FLOAT64; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_VX ] = 1; oiflag[ OCOL_VY ] = 1; oiflag[ CCOL_VX ] = 1; oiflag[ CCOL_VY ] = 1; columns_alloc_radec(p); break; case UI_KEY_GEOW1: name = gal_checkset_malloc_cat("GEO_", p->ctype[0]); unit = p->input->wcs->cunit[0]; ocomment = "Geometric center (WCS axis 1)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_FLOAT64; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_GX ] = 1; oiflag[ OCOL_GY ] = 1; ciflag[ CCOL_GX ] = 1; ciflag[ CCOL_GY ] = 1; columns_alloc_georadec(p); break; case UI_KEY_GEOW2: name = gal_checkset_malloc_cat("GEO_", p->ctype[1]); unit = p->input->wcs->cunit[1]; ocomment = "Geometric center (WCS axis 2)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_FLOAT64; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_GX ] = 1; oiflag[ OCOL_GY ] = 1; ciflag[ CCOL_GX ] = 1; ciflag[ CCOL_GY ] = 1; columns_alloc_georadec(p); break; case UI_KEY_CLUMPSW1: name = gal_checkset_malloc_cat("CLUMPS_", p->ctype[0]); unit = p->input->wcs->cunit[0]; ocomment = "Flux.wht center of all clumps (WCS axis 1)."; ccomment = NULL; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_C_VX ] = 1; oiflag[ OCOL_C_VY ] = 1; columns_alloc_clumpsradec(p); break; case UI_KEY_CLUMPSW2: name = gal_checkset_malloc_cat("CLUMPS_", p->ctype[1]); unit = p->input->wcs->cunit[1]; ocomment = "Flux.wht center of all clumps (WCS axis 2)."; ccomment = NULL; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 15; disp_precision = 7; oiflag[ OCOL_C_VX ] = 1; oiflag[ OCOL_C_VY ] = 1; columns_alloc_clumpsradec(p); break; case UI_KEY_CLUMPSGEOW1: name = gal_checkset_malloc_cat("CLUMPS_GEO", p->ctype[0]); unit = p->input->wcs->cunit[0]; ocomment = "Geometric center of all clumps (WCS axis 1)."; ccomment = NULL; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_C_GX ] = 1; oiflag[ OCOL_C_GY ] = 1; columns_alloc_clumpsgeoradec(p); break; case UI_KEY_CLUMPSGEOW2: name = gal_checkset_malloc_cat("CLUMPS_GEO", p->ctype[1]); unit = p->input->wcs->cunit[1]; ocomment = "Geometric center of all clumps (WCS axis 2)."; ccomment = NULL; otype = GAL_TYPE_FLOAT64; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 13; disp_precision = 7; oiflag[ OCOL_C_GX ] = 1; oiflag[ OCOL_C_GY ] = 1; columns_alloc_clumpsgeoradec(p); break; case UI_KEY_BRIGHTNESS: name = "BRIGHTNESS"; unit = p->input->unit ? p->input->unit : "pixelunit"; ocomment = "Brightness (sum of sky subtracted values)."; ccomment = "Brightness (sum of pixels subtracted by rivers)."; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 10; disp_precision = 4; oiflag[ OCOL_SUM ] = 1; ciflag[ CCOL_SUM ] = 1; ciflag[ CCOL_RIV_NUM ] = 1; ciflag[ CCOL_RIV_SUM ] = 1; break; case UI_KEY_CLUMPSBRIGHTNESS: name = "CLUMPS_BRIGHTNESS"; unit = p->input->unit ? p->input->unit : "pixelunit"; ocomment = "Brightness (sum of pixel values) in clumps."; ccomment = NULL; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 10; disp_precision = 4; oiflag[ OCOL_C_SUM ] = 1; break; case UI_KEY_NORIVERBRIGHTNESS: name = "NO_RIVER_BRIGHTNESS"; unit = p->input->unit ? p->input->unit : "pixelunit"; ocomment = NULL; ccomment = "Brightness (sum of sky subtracted values)."; otype = GAL_TYPE_INVALID; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 10; disp_precision = 4; ciflag[ CCOL_SUM ] = 1; break; case UI_KEY_MAGNITUDE: name = "MAGNITUDE"; unit = "log"; ocomment = "Magnitude."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 8; disp_precision = 3; oiflag[ OCOL_SUM ] = 1; ciflag[ CCOL_SUM ] = 1; p->hasmag = 1; break; case UI_KEY_MAGNITUDEERR: name = "MAGNITUDE_ERR"; unit = "log"; ocomment = "Error in measuring magnitude."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 8; disp_precision = 3; oiflag[ OCOL_SUMSTD ] = 1; oiflag[ OCOL_NUM ] = 1; oiflag[ OCOL_SUM ] = 1; ciflag[ CCOL_SUMSTD ] = 1; ciflag[ CCOL_NUM ] = 1; ciflag[ CCOL_SUM ] = 1; break; case UI_KEY_CLUMPSMAGNITUDE: name = "CLUMPS_MAGNITUDE"; unit = "log"; ocomment = "Magnitude in all clumps."; ccomment = NULL; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_INVALID; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 8; disp_precision = 3; oiflag[ OCOL_C_SUM ] = 1; p->hasmag = 1; break; case UI_KEY_UPPERLIMIT: name = "UPPERLIMIT"; unit = p->input->unit; ocomment = "Upper limit value (random positionings)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 8; disp_precision = 3; p->upperlimit = 1; /* Doesn't need per-pixel calculations. */ break; case UI_KEY_UPPERLIMITMAG: name = "UPPERLIMIT_MAG"; unit = "log"; ocomment = "Upper limit magnitude (random positionings)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 8; disp_precision = 3; p->upperlimit = 1; p->hasmag = 1; /* Doesn't need per-pixel calculations. */ break; case UI_KEY_RIVERAVE: name = "RIVER_AVE"; unit = p->input->unit ? p->input->unit : "pixelunit"; ocomment = NULL; ccomment = "Average river value surrounding this clump."; otype = GAL_TYPE_INVALID; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 10; disp_precision = 4; ciflag[ CCOL_RIV_NUM ] = 1; ciflag[ CCOL_RIV_SUM ] = 1; break; case UI_KEY_RIVERNUM: name = "RIVER_NUM"; unit = "counter"; ocomment = NULL; ccomment = "Number of river pixels around this clump."; otype = GAL_TYPE_INVALID; ctype = GAL_TYPE_INT32; disp_fmt = 0; disp_width = 5; disp_precision = 0; ciflag[ CCOL_RIV_NUM ] = 1; break; case UI_KEY_SN: name = "SN"; unit = "ratio"; ocomment = "Signal to noise ratio."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_SUMSTD ] = 1; oiflag[ OCOL_NUM ] = 1; oiflag[ OCOL_SUM ] = 1; ciflag[ CCOL_SUMSTD ] = 1; ciflag[ CCOL_NUM ] = 1; ciflag[ CCOL_SUM ] = 1; break; case UI_KEY_SKY: name = "SKY"; unit = p->input->unit ? p->input->unit : "pixelunit"; ocomment = "Average input sky value."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 10; disp_precision = 4; oiflag[ OCOL_NUM ] = 1; oiflag[ OCOL_SUMSKY ] = 1; ciflag[ CCOL_NUM ] = 1; ciflag[ CCOL_SUMSKY ] = 1; break; case UI_KEY_STD: name = "STD"; unit = p->input->unit ? p->input->unit : "pixelunit"; ocomment = "Average of input standard deviation."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_GENERAL; disp_width = 10; disp_precision = 4; oiflag[ OCOL_NUM ] = 1; oiflag[ OCOL_SUMSTD ] = 1; ciflag[ CCOL_NUM ] = 1; ciflag[ CCOL_SUMSTD ] = 1; break; case UI_KEY_SEMIMAJOR: name = "SEMI_MAJOR"; unit = "pixel"; ocomment = "Flux weighted semi-major axis."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_VXX ] = 1; oiflag[ OCOL_VYY ] = 1; oiflag[ OCOL_VXY ] = 1; ciflag[ CCOL_VXX ] = 1; ciflag[ CCOL_VYY ] = 1; ciflag[ CCOL_VXY ] = 1; break; case UI_KEY_SEMIMINOR: name = "SEMI_MINOR"; unit = "pixel"; ocomment = "Flux weighted semi-minor axis."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_VXX ] = 1; oiflag[ OCOL_VYY ] = 1; oiflag[ OCOL_VXY ] = 1; ciflag[ CCOL_VXX ] = 1; ciflag[ CCOL_VYY ] = 1; ciflag[ CCOL_VXY ] = 1; break; case UI_KEY_AXISRATIO: name = "AXIS_RATIO"; unit = "ratio"; ocomment = "Flux weighted axis ratio (minor/major)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 7; disp_precision = 3; oiflag[ OCOL_VXX ] = 1; oiflag[ OCOL_VYY ] = 1; oiflag[ OCOL_VXY ] = 1; ciflag[ CCOL_VXX ] = 1; ciflag[ CCOL_VYY ] = 1; ciflag[ CCOL_VXY ] = 1; break; case UI_KEY_POSITIONANGLE: name = "POSITION_ANGLE"; unit = "degrees"; ocomment = "Position angle."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_VXX ] = 1; oiflag[ OCOL_VYY ] = 1; oiflag[ OCOL_VXY ] = 1; ciflag[ CCOL_VXX ] = 1; ciflag[ CCOL_VYY ] = 1; ciflag[ CCOL_VXY ] = 1; break; case UI_KEY_GEOSEMIMAJOR: name = "GEO_SEMI_MAJOR"; unit = "pixel"; ocomment = "Geometric semi-major axis."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_GXX ] = 1; oiflag[ OCOL_GYY ] = 1; oiflag[ OCOL_GXY ] = 1; ciflag[ CCOL_GXX ] = 1; ciflag[ CCOL_GYY ] = 1; ciflag[ CCOL_GXY ] = 1; break; case UI_KEY_GEOSEMIMINOR: name = "GEO_SEMI_MINOR"; unit = "pixel"; ocomment = "Geometric semi-minor axis."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_GXX ] = 1; oiflag[ OCOL_GYY ] = 1; oiflag[ OCOL_GXY ] = 1; ciflag[ CCOL_GXX ] = 1; ciflag[ CCOL_GYY ] = 1; ciflag[ CCOL_GXY ] = 1; break; case UI_KEY_GEOAXISRATIO: name = "GEO_AXIS_RATIO"; unit = "ratio"; ocomment = "Geometric axis ratio (minor/major)."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 7; disp_precision = 3; oiflag[ OCOL_VXX ] = 1; oiflag[ OCOL_VYY ] = 1; oiflag[ OCOL_VXY ] = 1; ciflag[ CCOL_VXX ] = 1; ciflag[ CCOL_VYY ] = 1; ciflag[ CCOL_VXY ] = 1; break; case UI_KEY_GEOPOSITIONANGLE: name = "GEO_POSITION_ANGLE"; unit = "degrees"; ocomment = "Geometric Position angle."; ccomment = ocomment; otype = GAL_TYPE_FLOAT32; ctype = GAL_TYPE_FLOAT32; disp_fmt = GAL_TABLE_DISPLAY_FMT_FLOAT; disp_width = 10; disp_precision = 3; oiflag[ OCOL_GXX ] = 1; oiflag[ OCOL_GYY ] = 1; oiflag[ OCOL_GXY ] = 1; ciflag[ CCOL_GXX ] = 1; ciflag[ CCOL_GYY ] = 1; ciflag[ CCOL_GXY ] = 1; break; default: error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to fix " "the problem. The code %d is not an internally recognized " "column code", __func__, PACKAGE_BUGREPORT, colcode->v); } /* If this is an objects column, add it to the list of columns. We will be using the `status' element to keep the MakeCatalog code for the columns. */ if(otype!=GAL_TYPE_INVALID) { gal_list_data_add_alloc(&p->objectcols, NULL, otype, 1, &p->numobjects, NULL, 0, p->cp.minmapsize, name, unit, ocomment); p->objectcols->status = colcode->v; p->objectcols->disp_fmt = disp_fmt; p->objectcols->disp_width = disp_width; p->objectcols->disp_precision = disp_precision; } /* Similar to the objects column above but for clumps, but since the clumps image is optional, we need a further check before actually allocating the column. */ if(ctype!=GAL_TYPE_INVALID) { /* A clumps image has been given, so allocate space for this column. */ if(p->clumps) { gal_list_data_add_alloc(&p->clumpcols, NULL, ctype, 1, &p->numclumps, NULL, 0, p->cp.minmapsize, name, unit, ccomment); p->clumpcols->status = colcode->v; p->clumpcols->disp_fmt = disp_fmt; p->clumpcols->disp_width = disp_width; p->clumpcols->disp_precision = disp_precision; } /* If this is a clumps-only column and no clumps image was given. Add the column to the list of similar columns to inform the user. */ else if(otype==GAL_TYPE_INVALID) gal_list_str_add(&noclumpimg, name, 1); } } /* If a warning for clumps columns and no clumps image is necessary make the warning. */ if(noclumpimg) { gal_list_str_reverse(&noclumpimg); fprintf(stderr, "\n-------\n" "WARNING: the following column(s) are unique to " "clumps (not objects), but the objects image doesn't have " " `WCLUMPS' keyword. So these requested columns will be " "ignored.\n\n"); for(strtmp=noclumpimg; strtmp!=NULL; strtmp=strtmp->next) fprintf(stderr, "\t%s\n", strtmp->v); gal_list_str_free(noclumpimg, 1); fprintf(stderr, "\n-------\n"); } /* Free the general columns information because it is no longe needed, we'll set it back to NULL afterwards so it is not mistakenly used. */ gal_list_i32_free(p->columnids); p->columnids=NULL; } /******************************************************************/ /********** Column calculation ***************/ /******************************************************************/ #define MKC_RATIO(TOP,BOT) ( (BOT)!=0.0f ? (TOP)/(BOT) : NAN ) #define MKC_MAG(B) ( ((B)>0) ? -2.5f * log10(B) + p->zeropoint : NAN ) /* Calculate the Signal to noise ratio for the object. */ static double columns_sn(struct mkcatalogparams *p, double *row, int o0c1) { double var, sn, std, Ni, I, O; /* Get all the values as averages (per pixel). */ Ni = row[ o0c1 ? CCOL_NUM : OCOL_NUM ]; I = MKC_RATIO( row[ o0c1 ? CCOL_SUM : OCOL_SUM ], Ni ); std = MKC_RATIO( row[ o0c1 ? CCOL_SUMSTD : OCOL_SUMSTD ], Ni ); var = (p->skysubtracted ? 2.0f : 1.0f) * std * std; /* Calculate the S/N. Note that when grown clumps are requested from NoiseChisel, some "clumps" will completely cover their objects and there will be no rivers. So if this is a clump, and the river area is 0, we should treat the S/N as a an object. */ if( o0c1 && row[ CCOL_RIV_NUM ] ) { /* If the Sky is already subtracted, the varience should be counted two times. */ O = row[ CCOL_RIV_SUM ] / row[ CCOL_RIV_NUM ]; /* Outside. */ sn = ( (I-O)>0 ? ( sqrt(Ni/p->cpscorr) * (I-O) / sqrt( (I>0?I:-1*I) + (O>0?O:-1*O) + var ) ) : NAN ); } else sn = I>0 ? sqrt(Ni/p->cpscorr) * I / sqrt( (I>0?I:-1*I) + var ) : NAN; /* Return the derived value. */ return sn; } /* Do the second order calculations, see "Measuring elliptical parameters" section of the book/manual for a thorough explanation of the derivation. */ static double columns_second_order(struct mkcatalog_passparams *pp, double *row, int key, int o0c1) { double x=NAN, y=NAN, xx=NAN, yy=NAN, xy=NAN; double denom, kx=pp->shift[1]+1, ky=pp->shift[0]+1; /* Preparations. */ switch(key) { /* Brightness weighted. */ case UI_KEY_SEMIMAJOR: case UI_KEY_SEMIMINOR: case UI_KEY_POSITIONANGLE: /* Denominator (to be divided). */ denom = row[ o0c1 ? CCOL_SUMWHT : OCOL_SUMWHT ]; /* First order. */ x = MKC_RATIO( row[ o0c1 ? CCOL_VX : OCOL_VX ], denom ); y = MKC_RATIO( row[ o0c1 ? CCOL_VY : OCOL_VY ], denom ); /* Second order. */ xx = ( MKC_RATIO( row[ o0c1 ? CCOL_VXX : OCOL_VXX ], denom ) - (x-kx) * (x-kx) ); yy = ( MKC_RATIO( row[ o0c1 ? CCOL_VYY : OCOL_VYY ], denom ) - (y-ky) * (y-ky) ); xy = ( MKC_RATIO( row[ o0c1 ? CCOL_VXY : OCOL_VXY ], denom ) - (x-kx) * (y-ky) ); break; /* Geometric. */ case UI_KEY_GEOSEMIMAJOR: case UI_KEY_GEOSEMIMINOR: case UI_KEY_GEOPOSITIONANGLE: /* Denominator (to be divided). */ denom = row[ o0c1 ? CCOL_NUMALL : OCOL_NUMALL ]; /* First order. */ x = MKC_RATIO( row[ o0c1 ? CCOL_GX : OCOL_GX ], denom ); y = MKC_RATIO( row[ o0c1 ? CCOL_GY : OCOL_GY ], denom ); /* Second order. */ xx = ( MKC_RATIO( row[ o0c1 ? CCOL_GXX : OCOL_GXX ], denom ) - (x-kx) * (x-kx) ); yy = ( MKC_RATIO( row[ o0c1 ? CCOL_GYY : OCOL_GYY ], denom ) - (y-ky) * (y-ky) ); xy = ( MKC_RATIO( row[ o0c1 ? CCOL_GXY : OCOL_GXY ], denom ) - (x-kx) * (y-ky) ); break; /* Error. */ default: error(EXIT_FAILURE, 0, "%s: a bug! Code %d not a recognized key", __func__, key); } /* Return the output. */ switch(key) { /* Semi-major axis. */ case UI_KEY_SEMIMAJOR: case UI_KEY_GEOSEMIMAJOR: return sqrt( ( xx + yy ) / 2 + sqrt( (xx - yy)/2 * (xx - yy)/2 + xy * xy ) ); /* Semi-minor axis. */ case UI_KEY_SEMIMINOR: case UI_KEY_GEOSEMIMINOR: /*printf("\nhere\n");*/ return sqrt( ( xx + yy )/2 - sqrt( (xx - yy)/2 * (xx - yy)/2 + xy * xy ) ); /* Position angle. */ case UI_KEY_POSITIONANGLE: case UI_KEY_GEOPOSITIONANGLE: return 0.5f * atan2(2 * xy, xx - yy) * 180/M_PI; } /* Control should not reach here! If it does, its a bug, so abort and let the user know. */ error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s, so we can " "address the problem. Control should not have reached the end of " "this function", __func__, PACKAGE_BUGREPORT); return NAN; } /* The magnitude error is directly derivable from the S/N: To derive the error in measuring the magnitude from the S/N, let's take `F' as the flux, `Z' is the zeropoint, `M' is the magnitude, `S' is the S/N, and `D' to stand for capital delta (or error in a value) then from `M = -2.5*log10(F) + Z' we get the following equation after calculating the derivative with respect to F. `dM/df = -2.5 * ( 1 / ( F * ln(10) ) )' From the Tailor series, `DM' can be written as: `DM = dM/dF * DF' So `DM = |-2.5/ln(10)| * DF/F' But `DF/F' is just the inverse of the Signal to noise ratio, or `1/S'. So `DM = 2.5 / ( S * ln(10) )' */ #define MAG_ERROR(P,ROW,O0C1) (2.5f/(columns_sn((P),(ROW),(O0C1)) * log(10))) /* All the raw first and second pass information has been collected, now write them into the output columns. The list of columns here is in the same order as `columns_alloc_set_out_cols', see there for the type of each column. */ #define POS_V_G(ARRAY, SUMWHT_COL, NUMALL_COL, V_COL, G_COL) \ ( (ARRAY)[ SUMWHT_COL ]>0 \ ? MKC_RATIO( (ARRAY)[ V_COL ], (ARRAY)[ SUMWHT_COL ] ) \ : MKC_RATIO( (ARRAY)[ G_COL ], (ARRAY)[ NUMALL_COL ] ) ) void columns_fill(struct mkcatalog_passparams *pp) { struct mkcatalogparams *p=pp->p; int key; double tmp; void *colarr; gal_data_t *column; double *ci, *oi=pp->oi; size_t sr=pp->clumpstartindex, cind, coind; size_t oind=pp->object-1; /* IDs start from 1, indexs from 0. */ double **vo=NULL, **vc=NULL, **go=NULL, **gc=NULL, **vcc=NULL, **gcc=NULL; /* If a WCS column is requested (check will be done inside the function), then set the pointers. */ columns_set_wcs_pointers(p, &vo, &vc, &go, &gc, &vcc, &gcc); /* Go over all the object columns and fill in the information. */ for(column=p->objectcols; column!=NULL; column=column->next) { /* For easy reading. */ key=column->status; colarr=column->array; /* Go over all the columns. */ switch(key) { case UI_KEY_OBJID: ((int32_t *)colarr)[oind] = pp->object; break; case UI_KEY_NUMCLUMPS: ((int32_t *)colarr)[oind] = pp->clumpsinobj; break; case UI_KEY_AREA: ((int32_t *)colarr)[oind] = oi[OCOL_NUMALL]; break; case UI_KEY_CLUMPSAREA: ((int32_t *)colarr)[oind] = oi[OCOL_C_NUMALL]; break; case UI_KEY_WEIGHTAREA: ((int32_t *)colarr)[oind] = oi[OCOL_NUMWHT]; break; case UI_KEY_X: ((float *)colarr)[oind] = POS_V_G(oi, OCOL_SUMWHT, OCOL_NUMALL, OCOL_VX, OCOL_GX); break; case UI_KEY_Y: ((float *)colarr)[oind] = POS_V_G(oi, OCOL_SUMWHT, OCOL_NUMALL, OCOL_VY, OCOL_GY); break; case UI_KEY_GEOX: ((float *)colarr)[oind] = MKC_RATIO( oi[OCOL_GX], oi[OCOL_NUMALL] ); break; case UI_KEY_GEOY: ((float *)colarr)[oind] = MKC_RATIO( oi[OCOL_GY], oi[OCOL_NUMALL] ); break; case UI_KEY_CLUMPSX: ((float *)colarr)[oind] = POS_V_G(oi, OCOL_C_SUMWHT, OCOL_C_NUMALL, OCOL_C_VX, OCOL_C_GX); break; case UI_KEY_CLUMPSY: ((float *)colarr)[oind] = POS_V_G(oi, OCOL_C_SUMWHT, OCOL_C_NUMALL, OCOL_C_VY, OCOL_C_GY); break; case UI_KEY_CLUMPSGEOX: ((float *)colarr)[oind] = MKC_RATIO( oi[OCOL_C_GX], oi[OCOL_C_NUMALL] ); break; case UI_KEY_CLUMPSGEOY: ((float *)colarr)[oind] = MKC_RATIO( oi[OCOL_C_GY], oi[OCOL_C_NUMALL] ); break; case UI_KEY_W1: case UI_KEY_W2: vo[0][oind] = POS_V_G(oi, OCOL_SUMWHT, OCOL_NUMALL, OCOL_VX, OCOL_GX); vo[1][oind] = POS_V_G(oi, OCOL_SUMWHT, OCOL_NUMALL, OCOL_VY, OCOL_GY); break; case UI_KEY_GEOW1: case UI_KEY_GEOW2: go[0][oind] = MKC_RATIO( oi[OCOL_GX], oi[OCOL_NUMALL] ); go[1][oind] = MKC_RATIO( oi[OCOL_GY], oi[OCOL_NUMALL] ); break; case UI_KEY_CLUMPSW1: case UI_KEY_CLUMPSW2: vcc[0][oind] = POS_V_G(oi, OCOL_C_SUMWHT, OCOL_C_NUMALL, OCOL_C_VX, OCOL_C_GX); vcc[1][oind] = POS_V_G(oi, OCOL_C_SUMWHT, OCOL_C_NUMALL, OCOL_C_VY, OCOL_C_GY); break; case UI_KEY_CLUMPSGEOW1: case UI_KEY_CLUMPSGEOW2: gcc[0][oind] = MKC_RATIO( oi[OCOL_C_GX], oi[OCOL_C_NUMALL] ); gcc[1][oind] = MKC_RATIO( oi[OCOL_C_GY], oi[OCOL_C_NUMALL] ); break; case UI_KEY_BRIGHTNESS: ((float *)colarr)[oind] = ( oi[ OCOL_NUM ]>0.0f ? oi[ OCOL_SUM ] : NAN ); break; case UI_KEY_CLUMPSBRIGHTNESS: ((float *)colarr)[oind] = ( oi[ OCOL_C_NUM ]>0.0f ? oi[ OCOL_C_SUM ] : NAN ); break; case UI_KEY_MAGNITUDE: ((float *)colarr)[oind] = MKC_MAG(oi[ OCOL_SUM ]); break; case UI_KEY_MAGNITUDEERR: ((float *)colarr)[oind] = MAG_ERROR(p, oi, 0); break; case UI_KEY_CLUMPSMAGNITUDE: ((float *)colarr)[oind] = MKC_MAG(oi[ OCOL_C_SUM ]); break; case UI_KEY_UPPERLIMIT: ((float *)colarr)[oind] = oi[ OCOL_UPPERLIMIT_B ]; break; case UI_KEY_UPPERLIMITMAG: ((float *)colarr)[oind] = MKC_MAG(oi[ OCOL_UPPERLIMIT_B ]); break; case UI_KEY_SN: ((float *)colarr)[oind] = columns_sn(p, oi, 0); break; case UI_KEY_SKY: ((float *)colarr)[oind] = MKC_RATIO(oi[OCOL_SUMSKY], oi[OCOL_NUM]); break; case UI_KEY_STD: ((float *)colarr)[oind] = MKC_RATIO(oi[OCOL_SUMSTD], oi[OCOL_NUM]); break; case UI_KEY_SEMIMAJOR: ((float *)colarr)[oind] = columns_second_order(pp, oi, key, 0); break; case UI_KEY_SEMIMINOR: ((float *)colarr)[oind] = columns_second_order(pp, oi, key, 0); break; case UI_KEY_AXISRATIO: ((float *)colarr)[oind] = ( columns_second_order(pp, oi, UI_KEY_SEMIMINOR, 0) / columns_second_order(pp, oi, UI_KEY_SEMIMAJOR, 0) ); break; case UI_KEY_POSITIONANGLE: ((float *)colarr)[oind] = columns_second_order(pp, oi, key, 0); break; case UI_KEY_GEOSEMIMAJOR: ((float *)colarr)[oind] = columns_second_order(pp, oi, key, 0); break; case UI_KEY_GEOSEMIMINOR: ((float *)colarr)[oind] = columns_second_order(pp, oi, key, 0); break; case UI_KEY_GEOAXISRATIO: ((float *)colarr)[oind] = ( columns_second_order(pp, oi, UI_KEY_GEOSEMIMINOR, 0) / columns_second_order(pp, oi, UI_KEY_GEOSEMIMAJOR, 0) ); break; case UI_KEY_GEOPOSITIONANGLE: ((float *)colarr)[oind] = columns_second_order(pp, oi, key, 0); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " "solve the problem. the output column code %d not recognized " "(for objects). ", __func__, PACKAGE_BUGREPORT, key); } } /* Go over the clump columns and fill the information. */ for(column=p->clumpcols; column!=NULL; column=column->next) for(coind=0;coind<pp->clumpsinobj;++coind) { /* `coind': clump-in-object-index. `cind': clump-index (over all the catalog). */ cind = sr + coind; colarr = column->array; key = column->status; ci = &pp->ci[ coind * CCOL_NUMCOLS ]; /* Parse columns */ switch(key) { case UI_KEY_HOSTOBJID: ((int32_t *)colarr)[cind]=pp->object; break; case UI_KEY_IDINHOSTOBJ: ((int32_t *)colarr)[cind]=coind+1; break; case UI_KEY_AREA: ((int32_t *)colarr)[cind]=ci[CCOL_NUMALL]; break; case UI_KEY_WEIGHTAREA: ((int32_t *)colarr)[cind]=ci[CCOL_NUMWHT]; break; case UI_KEY_X: ((float *)colarr)[cind] = POS_V_G(ci, CCOL_SUMWHT, CCOL_NUMALL, CCOL_VX, CCOL_GX); break; case UI_KEY_Y: ((float *)colarr)[cind] = POS_V_G(ci, CCOL_SUMWHT, CCOL_NUMALL, CCOL_VY, CCOL_GY); break; case UI_KEY_GEOX: ((float *)colarr)[cind] = MKC_RATIO( ci[CCOL_GX], ci[CCOL_NUMALL] ); break; case UI_KEY_GEOY: ((float *)colarr)[cind] = MKC_RATIO( ci[CCOL_GY], ci[CCOL_NUMALL] ); break; case UI_KEY_W1: case UI_KEY_W2: vc[0][cind] = POS_V_G(ci, CCOL_SUMWHT, CCOL_NUMALL, CCOL_VX, CCOL_GX); vc[1][cind] = POS_V_G(ci, CCOL_SUMWHT, CCOL_NUMALL, CCOL_VY, CCOL_GY); break; case UI_KEY_GEOW1: case UI_KEY_GEOW2: gc[0][cind] = MKC_RATIO( ci[CCOL_GX], ci[CCOL_NUMALL] ); gc[1][cind] = MKC_RATIO( ci[CCOL_GY], ci[CCOL_NUMALL] ); break; case UI_KEY_BRIGHTNESS: /* Calculate the river flux over the clump area. But only when rivers are present. When grown clumps are requested, the clumps can fully cover a detection (that has one or no clumps). */ tmp = ( ci[ CCOL_RIV_NUM ]>0.0f ? ci[ CCOL_RIV_SUM ]/ci[ CCOL_RIV_NUM ]*ci[ CCOL_NUM ] : 0 ); /* Subtract it from the clump's brightness. */ ((float *)colarr)[cind] = ( ci[ CCOL_NUM ]>0.0f ? (ci[ CCOL_SUM ] - tmp) : NAN ); break; case UI_KEY_NORIVERBRIGHTNESS: ((float *)colarr)[cind] = ( ci[ CCOL_NUM ]>0.0f ? ci[ CCOL_SUM ] : NAN ); break; case UI_KEY_MAGNITUDE: /* Similar: brightness for clumps */ tmp = ( ci[ CCOL_RIV_NUM ] ? ci[ CCOL_RIV_SUM ]/ci[ CCOL_RIV_NUM ]*ci[ CCOL_NUM ] : 0 ); ((float *)colarr)[cind] = MKC_MAG(ci[ CCOL_SUM ]-tmp); break; case UI_KEY_MAGNITUDEERR: ((float *)colarr)[cind] = MAG_ERROR(p, ci, 1); break; case UI_KEY_UPPERLIMIT: ((float *)colarr)[cind] = ci[ CCOL_UPPERLIMIT_B ]; break; case UI_KEY_UPPERLIMITMAG: ((float *)colarr)[cind] = MKC_MAG(ci[ CCOL_UPPERLIMIT_B ]); break; case UI_KEY_RIVERAVE: ((float *)colarr)[cind] = ( ci[ CCOL_RIV_NUM] ? ci[ CCOL_RIV_SUM ]/ci[ CCOL_RIV_NUM] : NAN ); break; case UI_KEY_RIVERNUM: ((int32_t *)colarr)[cind] = ci[ CCOL_RIV_NUM ]; break; case UI_KEY_SN: ((float *)colarr)[cind] = columns_sn(p, ci, 1); break; case UI_KEY_SKY: ((float *)colarr)[cind] = MKC_RATIO( ci[ CCOL_SUMSKY], ci[ CCOL_NUM] ); break; case UI_KEY_STD: ((float *)colarr)[cind] = MKC_RATIO( ci[ CCOL_SUMSTD ], ci[ CCOL_NUM ] ); break; case UI_KEY_SEMIMAJOR: ((float *)colarr)[cind] = columns_second_order(pp, ci, key, 1); break; case UI_KEY_SEMIMINOR: ((float *)colarr)[cind] = columns_second_order(pp, ci, key, 1); break; case UI_KEY_AXISRATIO: ((float *)colarr)[cind] = ( columns_second_order(pp, ci, UI_KEY_SEMIMINOR, 1) / columns_second_order(pp, ci, UI_KEY_SEMIMAJOR, 1) ); break; case UI_KEY_POSITIONANGLE: ((float *)colarr)[cind] = columns_second_order(pp, ci, key, 1); break; case UI_KEY_GEOSEMIMAJOR: ((float *)colarr)[cind] = columns_second_order(pp, ci, key, 1); break; case UI_KEY_GEOSEMIMINOR: ((float *)colarr)[cind] = columns_second_order(pp, ci, key, 1); break; case UI_KEY_GEOAXISRATIO: ((float *)colarr)[cind] = ( columns_second_order(pp, ci, UI_KEY_GEOSEMIMINOR, 1) / columns_second_order(pp, ci, UI_KEY_GEOSEMIMAJOR, 1) ); break; case UI_KEY_GEOPOSITIONANGLE: ((float *)colarr)[cind] = columns_second_order(pp, ci, key, 1); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " "solve the problem. The output column code %d not " "recognized (for clumps). ", __func__, PACKAGE_BUGREPORT, key); } } /* Clean up. */ if(vo) free(vo); if(vc) free(vc); if(go) free(go); if(gc) free(gc); if(vcc) free(vcc); if(gcc) free(gcc); } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/mkcatalog.c��������������������������������������������������������������0000644�0001750�0001750�00000075532�13216276304�015001� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <float.h> #include <string.h> #include <stdlib.h> #include <inttypes.h> #include <gnuastro/git.h> #include <gnuastro/wcs.h> #include <gnuastro/data.h> #include <gnuastro/fits.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "mkcatalog.h" #include "ui.h" #include "columns.h" #include "upperlimit.h" /*********************************************************************/ /************* Definitions and initialization ***************/ /*********************************************************************/ /* Both passes are going to need their starting pointers set, so we'll do that here. */ static void mkcatalog_initialize_params(struct mkcatalog_passparams *pp) { struct mkcatalogparams *p=pp->p; /* Initialize the number of clumps in this object. */ pp->clumpsinobj=0; /* Initialize the intermediate values. */ memset(pp->oi, 0, OCOL_NUMCOLS * sizeof *pp->oi); /* Set the shifts in every dimension to avoid round-off errors in large numbers for the non-linear calculations. We are using the first pixel of each object's tile as the shift parameter to keep the mean (average) reasonably near to the standard deviation. Otherwise, when the object is far out in the image (large x and y positions), then roundoff errors are going to decrease the accuracy of the second order calculations. */ gal_dimension_index_to_coord( ( (float *)(pp->tile->array) - (float *)(pp->tile->block->array) ), p->input->ndim, p->input->dsize, pp->shift); /* Set the starting and ending indexs of this tile/object. */ pp->st_i = gal_tile_start_end_ind_inclusive(pp->tile, p->input, pp->start_end_inc); pp->st_sky = (float *)(p->sky->array) + pp->start_end_inc[0]; pp->st_std = (float *)(p->std->array) + pp->start_end_inc[0]; pp->st_o = (int32_t *)(p->objects->array) + pp->start_end_inc[0]; pp->st_c = ( p->clumps ? (int32_t *)(p->clumps->array) + pp->start_end_inc[0] : NULL ); } /*********************************************************************/ /************* First and second passes ***************/ /*********************************************************************/ static void mkcatalog_first_pass(struct mkcatalog_passparams *pp) { struct mkcatalogparams *p=pp->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; double *oi=pp->oi; int32_t *O, *C=NULL; size_t d, increment=0, num_increment=1; float ss, *I, *II, *SK, *ST, *input=p->input->array; size_t *c=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "c"); size_t *sc=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "sc"); /* Parse each contiguous patch of memory covered by this object. */ while( pp->start_end_inc[0] + increment <= pp->start_end_inc[1] ) { /* Set the contiguous range to parse, we will check the count over the `I' pointer and just increment the rest. */ O = pp->st_o + increment; SK = pp->st_sky + increment; ST = pp->st_std + increment; if(p->clumps) C = pp->st_c + increment; II = ( I = pp->st_i + increment ) + pp->tile->dsize[ndim-1]; /* Parse the tile. */ do { /* If this pixel belongs to the requested object then do the processing. */ if( *O==pp->object ) { /* Get the number of clumps in this object: the largest clump ID over each object. */ if( p->clumps && *C>0 ) pp->clumpsinobj = *C > pp->clumpsinobj ? *C : pp->clumpsinobj; /* Get the coordinates of this point. */ gal_dimension_index_to_coord(I-input, ndim, dsize, c); /* Calculate the shifted coordinates for second order calculations. The coordinate is incremented because from now on, the positions are in the FITS standard (starting from one). IMPORTANT NOTE: this is a postfix increment, so after the expression (difference) is evaluated, the coordinate is going to change. This is necessary because `shift' is also starting from zero. */ for(d=0;d<ndim;++d) sc[d] = c[d]++ - pp->shift[d]; /* Do the general geometric (independent of pixel value) calculations. */ oi[ OCOL_NUMALL ]++; oi[ OCOL_GX ] += c[1]; oi[ OCOL_GY ] += c[0]; oi[ OCOL_GXX ] += sc[1] * sc[1]; oi[ OCOL_GYY ] += sc[0] * sc[0]; oi[ OCOL_GXY ] += sc[1] * sc[0]; if(p->clumps && *C>0) { oi[ OCOL_C_GX ] += c[1]; oi[ OCOL_C_GY ] += c[0]; } /* Start the pixel value related parameters. ABOUT THE CHECK: The reason this condition is given like this is that the `threshold' value is optional and we don't want to do multiple checks. The basic idea is this: when the user doesn't want any thresholds applied, then `p->threshold==NAN' and any conditional that involves a NaN will fail, so its logical negation will be positive and the calculations below will be done. However, if the user does specify a threhold and the pixel is above the threshold, then (`ss < p->threshold * *ST') will be false and its logical negation will be positive, so the pixel will be included. */ if( !( p->hasblank && isnan(*I) ) && !( (ss = *I - *SK) < p->threshold * *ST ) ) { /* General flux summations. */ oi[ OCOL_NUM ]++; oi[ OCOL_SUM ] += ss; oi[ OCOL_SUMSKY ] += *SK; oi[ OCOL_SUMSTD ] += *ST; if(p->clumps && *C>0) { oi[ OCOL_C_NUM ]++; oi[ OCOL_C_SUM ] += ss; } /* For flux weighted centers, we can only use positive values, so do those measurements here. */ if( ss > 0.0f ) { oi[ OCOL_NUMWHT ]++; oi[ OCOL_SUMWHT ] += ss; oi[ OCOL_VX ] += ss * c[1]; oi[ OCOL_VY ] += ss * c[0]; oi[ OCOL_VXX ] += ss * sc[1] * sc[1]; oi[ OCOL_VYY ] += ss * sc[0] * sc[0]; oi[ OCOL_VXY ] += ss * sc[1] * sc[0]; if(p->clumps && *C>0) { oi[ OCOL_C_NUMWHT ]++; oi[ OCOL_C_SUMWHT ] += ss; oi[ OCOL_C_VX ] += ss * c[1]; oi[ OCOL_C_VY ] += ss * c[0]; } } } } /* Increment the other pointers. */ ++O; ++SK; ++ST; if(p->clumps) ++C; } while(++I<II); /* Increment to the next contiguous region of this tile. */ increment += ( gal_tile_block_increment(p->input, dsize, num_increment++, NULL) ); } /* Clean up. */ free(c); free(sc); } /* Do the second pass */ static void mkcatalog_second_pass(struct mkcatalog_passparams *pp) { struct mkcatalogparams *p=pp->p; size_t ndim=p->input->ndim, *dsize=p->input->dsize; double *ci; int32_t *O, *C=NULL, nlab, *ngblabs; size_t i, ii, d, increment=0, num_increment=1; size_t nngb=gal_dimension_num_neighbors(ndim); size_t *dinc=gal_dimension_increment(ndim, dsize); float ss, *I, *II, *SK, *ST, *input=p->input->array; int32_t *objects=p->objects->array, *clumps=p->clumps->array; size_t *c=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "c"); size_t *sc=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "sc"); /* Allocate array to keep the neighbor labels. */ ngblabs=gal_data_malloc_array(GAL_TYPE_INT32, nngb, __func__, "ngblabs"); /* Parse each contiguous patch of memory covered by this object. */ while( pp->start_end_inc[0] + increment <= pp->start_end_inc[1] ) { /* Set the contiguous range to parse, we will check the count over the `I' pointer and just increment the rest. */ O = pp->st_o + increment; SK = pp->st_sky + increment; ST = pp->st_std + increment; if(p->clumps) C = pp->st_c + increment; II = ( I = pp->st_i + increment ) + pp->tile->dsize[ndim-1]; /* Parse the next contiguous region of this tile. */ do { /* If this pixel belongs to the requested object, is a clumps and isn't NAN, then do the processing. `hasblank' is constant, so when the input doesn't have any blank values, the `isnan' will never be checked. */ if( *O==pp->object ) { /* We are on a clump. */ if(p->clumps && *C>0) { /* Pointer to make things easier. Note that the clump labels start from 1, but the array indexs from 0.*/ ci=&pp->ci[ (*C-1) * CCOL_NUMCOLS ]; /* Get the coordinates of this point. */ gal_dimension_index_to_coord(I-input, ndim, dsize, c); /* Shifted coordinates for second order moments, see explanations in the first pass.*/ for(d=0;d<ndim;++d) sc[d] = c[d]++ - pp->shift[d]; /* Geometric measurements (independent of pixel value). */ ci[ CCOL_NUMALL ]++; ci[ CCOL_GX ] += c[1]; ci[ CCOL_GY ] += c[0]; ci[ CCOL_GXX ] += sc[1] * sc[1]; ci[ CCOL_GYY ] += sc[0] * sc[0]; ci[ CCOL_GXY ] += sc[1] * sc[0]; /* Only use pixels above the threshold, see explanations in first pass for an explanation. */ if( !( p->hasblank && isnan(*I) ) && !( (ss = *I - *SK) < p->threshold * *ST ) ) { /* Fill in the necessary information. */ ci[ CCOL_NUM ]++; ci[ CCOL_SUM ] += ss; ci[ CCOL_SUMSKY ] += *SK; ci[ CCOL_SUMSTD ] += *ST; if( ss > 0.0f ) { ci[ CCOL_NUMWHT ]++; ci[ CCOL_SUMWHT ] += ss; ci[ CCOL_VX ] += ss * c[1]; ci[ CCOL_VY ] += ss * c[0]; ci[ CCOL_VXX ] += ss * sc[1] * sc[1]; ci[ CCOL_VYY ] += ss * sc[0] * sc[0]; ci[ CCOL_VXY ] += ss * sc[1] * sc[0]; } } } /* This pixel is on the diffuse region, check to see if it is touching a clump or not, but only if this object actually has any clumps. */ else if(pp->clumpsinobj) { /* We are on a diffuse (possibly a river) pixel. So the value of this pixel has to be added to any of the clumps in touches. But since it might touch a labeled region more than once, we use `ngblabs' to keep track of which label we have already added its value to. `ii' is the number of different labels this river pixel has already been considered for. `ngblabs' will keep the list labels. */ ii=0; memset(ngblabs, 0, nngb*sizeof *ngblabs); /* Go over the neighbors and see if this pixel is touching a clump or not. */ GAL_DIMENSION_NEIGHBOR_OP(I-input, ndim, dsize, ndim, dinc, { /* Neighbor's label (mainly for easy reading). */ nlab=clumps[nind]; /* We only want neighbors that are a clump and part of this object and part of the same object. */ if( nlab>0 && objects[nind]==pp->object) { /* Go over all already checked labels and make sure this clump hasn't already been considered. */ for(i=0;i<ii;++i) if(ngblabs[i]==nlab) break; /* It hasn't been considered yet: */ if(i==ii) { ngblabs[ii++] = nlab; ++(pp->ci)[ (nlab-1) * CCOL_NUMCOLS + CCOL_RIV_NUM ]; pp->ci[ (nlab-1) * CCOL_NUMCOLS + CCOL_RIV_SUM ] += *I-*SK; } } }); } } /* Increment the other pointers. */ ++O; ++SK; ++ST; if(p->clumps) ++C; } while(++I<II); /* Increment to the next contiguous region of this tile. */ increment += ( gal_tile_block_increment(p->input, dsize, num_increment++, NULL) ); } /* Clean up. */ free(c); free(sc); free(dinc); free(ngblabs); } /*********************************************************************/ /***************** High-level funcitons *******************/ /*********************************************************************/ static void mkcatalog_clump_starting_index(struct mkcatalog_passparams *pp) { struct mkcatalogparams *p=pp->p; /* Lock the mutex if we are working on more than one thread. NOTE: it is very important to keep the number of operations within the mutex to a minimum so other threads don't get delayed. */ if(p->cp.numthreads>1) pthread_mutex_lock(&p->mutex); /* Put the current total number of rows filled into the output, then increment the total number by the number of clumps. */ pp->clumpstartindex = p->clumprowsfilled; p->clumprowsfilled += pp->clumpsinobj; /* Unlock the mutex (if it was locked). */ if(p->cp.numthreads>1) pthread_mutex_unlock(&p->mutex); } /* Each thread will call this function once. It will go over all the objects that are assigned to it. */ static void * mkcatalog_single_object(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct mkcatalogparams *p=(struct mkcatalogparams *)(tprm->params); size_t ndim=p->input->ndim; size_t i; struct mkcatalog_passparams pp; /* Initialize the mkcatalog_passparams elements. */ pp.p = p; pp.clumpstartindex = 0; pp.rng = p->rng ? gsl_rng_clone(p->rng) : NULL; pp.shift = gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "pp.shift"); pp.oi = gal_data_malloc_array(GAL_TYPE_FLOAT64, OCOL_NUMCOLS, __func__, "pp.oi"); /* If we have upper-limit mode, then allocate the container to keep the values to calculate the standard deviation. */ pp.up_vals = p->upperlimit ? gal_data_alloc(NULL, GAL_TYPE_FLOAT32, 1, &p->upnum, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL) : NULL; /* Fill the desired columns for all the objects given to this thread. */ for(i=0; tprm->indexs[i]!=GAL_BLANK_SIZE_T; ++i) { /* For easy reading, Note that the object IDs start from one while the array positions start from 0. */ pp.ci=NULL; pp.object = tprm->indexs[i] + 1; pp.tile = &p->tiles[ tprm->indexs[i] ]; /* Initialize the parameters for this object/tile. */ mkcatalog_initialize_params(&pp); /* Get the first pass information. */ mkcatalog_first_pass(&pp); /* Currently the second pass is only necessary when there is a clumps image. */ if(p->clumps) { /* Allocate space for the properties of each clump. */ pp.ci = gal_data_calloc_array(GAL_TYPE_FLOAT64, pp.clumpsinobj * CCOL_NUMCOLS, __func__, "pp.ci"); /* Get the starting row of this object's clumps in the final catalog. This index is also necessary for the unique random number generator seeds of each clump. */ mkcatalog_clump_starting_index(&pp); /* Get the second pass information. */ mkcatalog_second_pass(&pp); } /* Calculate the upper limit magnitude (if necessary). */ if(p->upperlimit) upperlimit_calculate(&pp); /* Write the pass information into the columns. */ columns_fill(&pp); /* Clean up for this object. */ if(pp.ci) free(pp.ci); } /* Clean up. */ free(pp.oi); free(pp.shift); gal_data_free(pp.up_vals); if(pp.rng) gsl_rng_free(pp.rng); /* Wait until all the threads finish and return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } /*********************************************************************/ /******** Processing after threads finish *************/ /*********************************************************************/ /* Convert internal image coordinates to WCS for table. Note that from the beginning (during the passing steps), we saved FITS coordinates. Also note that we are doing the conversion in place. */ static void mkcatalog_wcs_conversion(struct mkcatalogparams *p) { gal_data_t *c; gal_data_t *column; /* Flux weighted center positions for clumps and objects. */ if(p->wcs_vo) { gal_wcs_img_to_world(p->wcs_vo, p->input->wcs, 1); if(p->wcs_vc) gal_wcs_img_to_world(p->wcs_vc, p->input->wcs, 1); } /* Geometric center positions for clumps and objects. */ if(p->wcs_go) { gal_wcs_img_to_world(p->wcs_go, p->input->wcs, 1); if(p->wcs_gc) gal_wcs_img_to_world(p->wcs_gc, p->input->wcs, 1); } /* All clumps flux weighted center. */ if(p->wcs_vcc) gal_wcs_img_to_world(p->wcs_vcc, p->input->wcs, 1); /* All clumps geometric center. */ if(p->wcs_gcc) gal_wcs_img_to_world(p->wcs_gcc, p->input->wcs, 1); /* Go over all the object columns and fill in the values. */ for(column=p->objectcols; column!=NULL; column=column->next) { /* Definitions */ c=NULL; /* Set `c' for the columns that must be corrected. Note that this `switch' statement doesn't need any `default', because there are probably columns that don't need any correction. */ switch(column->status) { case UI_KEY_W1: c=p->wcs_vo; break; case UI_KEY_W2: c=p->wcs_vo->next; break; case UI_KEY_GEOW1: c=p->wcs_go; break; case UI_KEY_GEOW2: c=p->wcs_go->next; break; case UI_KEY_CLUMPSW1: c=p->wcs_vcc; break; case UI_KEY_CLUMPSW2: c=p->wcs_vcc->next; break; case UI_KEY_CLUMPSGEOW1: c=p->wcs_gcc; break; case UI_KEY_CLUMPSGEOW2: c=p->wcs_gcc->next; break; } /* Copy the elements into the output column. */ if(c) memcpy(column->array, c->array, column->size*gal_type_sizeof(c->type)); } /* Go over all the clump columns and fill in the values. */ for(column=p->clumpcols; column!=NULL; column=column->next) { /* Definitions */ c=NULL; /* Set `c' for the columns that must be corrected. Note that this `switch' statement doesn't need any `default', because there are probably columns that don't need any correction. */ switch(column->status) { case UI_KEY_W1: c=p->wcs_vc; break; case UI_KEY_W2: c=p->wcs_vc->next; break; case UI_KEY_GEOW1: c=p->wcs_gc; break; case UI_KEY_GEOW2: c=p->wcs_gc->next; break; } /* Copy the elements into the output column. */ if(c) memcpy(column->array, c->array, column->size*gal_type_sizeof(c->type)); } } /* Write the similar information. */ static gal_list_str_t * mkcatalog_outputs_same_start(struct mkcatalogparams *p, int o0c1, char *ObjClump) { float snlim; char *str, *tstr; double pixarea=NAN; gal_list_str_t *comments=NULL; char *skyfile=p->skyfile ? p->skyfile : p->inputname; char *stdfile=p->stdfile ? p->stdfile : p->inputname; char *clumpsfile=p->clumpsfile ? p->clumpsfile : p->inputname; char *objectsfile=p->objectsfile ? p->objectsfile : p->inputname; asprintf(&str, "%s catalog of %s", o0c1 ? "Object" : "Clump", PROGRAM_STRING); gal_list_str_add(&comments, str, 0); /* If in a Git controlled directory and output isn't a FITS file (in FITS, this will be automatically included). */ if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT && gal_git_describe()) { asprintf(&str, "Working directory commit %s", gal_git_describe()); gal_list_str_add(&comments, str, 0); } /* Write the date. However, `ctime' is going to put a new-line character in the end of its string, so we are going to remove it manually. */ asprintf(&str, "%s started on %s", PROGRAM_NAME, ctime(&p->rawtime)); str[strlen(str)-1]='\0'; gal_list_str_add(&comments, str, 0); if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) { asprintf(&str, "--------- Input files ---------"); gal_list_str_add(&comments, str, 0); } asprintf(&str, "Values: %s (hdu: %s).", p->inputname, p->cp.hdu); gal_list_str_add(&comments, str, 0); asprintf(&str, "Objects: %s (hdu: %s).", objectsfile, p->objectshdu); gal_list_str_add(&comments, str, 0); if(p->clumps) { asprintf(&str, "Clumps: %s (hdu: %s).", clumpsfile, p->clumpshdu); gal_list_str_add(&comments, str, 0); } asprintf(&str, "Sky: %s (hdu: %s).", skyfile, p->skyhdu); gal_list_str_add(&comments, str, 0); asprintf(&str, "Sky STD: %s (hdu: %s).", stdfile, p->stdhdu); gal_list_str_add(&comments, str, 0); if(p->upmaskfile) { asprintf(&str, "Upperlimit mask: %s (hdu: %s).", p->upmaskfile, p->upmaskhdu); gal_list_str_add(&comments, str, 0); } if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) { asprintf(&str, "--------- Supplimentary information ---------"); gal_list_str_add(&comments, str, 0); } if(p->input->wcs) { pixarea=gal_wcs_pixel_area_arcsec2(p->input->wcs); if( isnan(pixarea)==0 ) { asprintf(&str, "Pixel area (arcsec^2): %g", pixarea); gal_list_str_add(&comments, str, 0); } } if(p->hasmag) { asprintf(&str, "Zeropoint magnitude: %.4f", p->zeropoint); gal_list_str_add(&comments, str, 0); } /* Print surface brightness limits. */ if( !isnan(p->zeropoint) && !isnan(p->sfmagnsigma) ) { /* Per pixel. */ asprintf(&str, "%g sigma surface brightness (magnitude/pixel): %.3f", p->sfmagnsigma, ( -2.5f *log10( p->sfmagnsigma * p->medstd ) + p->zeropoint ) ); gal_list_str_add(&comments, str, 0); /* Per requested projected area: if a pixel area could be measured (a WCS was given), then also estimate the surface brightness over one arcsecond^2. From the pixel area, we know how many pixels are necessary to fill the requested projected area (in arcsecond^2). We also know that as the number of samples (pixels) increases (to N), the noise increases by sqrt(N), see the full discussion in the book. */ if(!isnan(pixarea) && !isnan(p->sfmagarea)) { /* Prepare the comment/information. */ if(p->sfmagarea==1.0f) tstr=NULL; else asprintf(&tstr, "%g-", p->sfmagarea); asprintf(&str, "%g sigma surface brightness (magnitude/%sarcsec^2): " "%.3f", p->sfmagnsigma, tstr ? tstr : "", ( -2.5f * log10( p->sfmagnsigma * p->medstd * sqrt( p->sfmagarea / pixarea) ) + p->zeropoint ) ); /* Add the final string/line to the catalog comments. */ gal_list_str_add(&comments, str, 0); /* Clean up (if necessary). */ if (tstr) { free(tstr); tstr=NULL; } } /* Notice: */ asprintf(&str, "Pixel STD for surface brightness calculation%s: %f", (!isnan(pixarea) && !isnan(p->sfmagarea))?"s":"", p->medstd); gal_list_str_add(&comments, str, 0); } snlim = o0c1 ? p->clumpsn : p->detsn; if( !isnan(snlim) ) { asprintf(&str, "%s limiting signal-to-noise ratio: %.3f", ObjClump, snlim); gal_list_str_add(&comments, str, 0); } if(o0c1==0) { asprintf(&str, "(NOTE: S/N limit above is for pseudo-detections, " "not objects.)"); gal_list_str_add(&comments, str, 0); } if(p->cpscorr>1.0f) { asprintf(&str, "Counts-per-second correction: %.3f", p->cpscorr); gal_list_str_add(&comments, str, 0); } if( !isnan(p->threshold) ) { asprintf(&str, "**IMPORTANT** Pixel threshold (multiple of local " "std): %.3f", p->threshold); gal_list_str_add(&comments, str, 0); } if(p->upperlimit) { if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) { asprintf(&str, "--------- Upper-limit measurement ---------"); gal_list_str_add(&comments, str, 0); } asprintf(&str, "Number of random samples: %zu", p->upnum); gal_list_str_add(&comments, str, 0); if(p->uprange) { asprintf(&str, "Range of random samples about target: %zu, %zu", p->uprange[1], p->uprange[0]); gal_list_str_add(&comments, str, 0); } asprintf(&str, "Random number generator name: %s", p->rngname); gal_list_str_add(&comments, str, 0); asprintf(&str, "Random number generator seed: %"PRIu64, p->seed); gal_list_str_add(&comments, str, 0); asprintf(&str, "Multiple of STD used for sigma-clipping: %.3f", p->upsigmaclip[0]); gal_list_str_add(&comments, str, 0); if(p->upsigmaclip[1]>=1.0f) asprintf(&str, "Number of clips for sigma-clipping: %.0f", p->upsigmaclip[1]); else asprintf(&str, "Tolerance level to sigma-clipping: %.3f", p->upsigmaclip[1]); gal_list_str_add(&comments, str, 0); asprintf(&str, "Multiple of sigma-clipped STD for upper-limit: %.3f", p->upnsigma); gal_list_str_add(&comments, str, 0); } if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) { asprintf(&str, "--------- Table columns ---------"); gal_list_str_add(&comments, str, 0); } /* Return the comments. */ return comments; } /* Write the produced columns into the output */ static void mkcatalog_write_outputs(struct mkcatalogparams *p) { /*char *str;*/ gal_list_str_t *comments; /* OBJECT CATALOG ============== */ comments=mkcatalog_outputs_same_start(p, 0, "Detection"); /* Write objects catalog --------------------- Reverse the comments list (so it is printed in the same order here), write the objects catalog and free the comments. */ gal_list_str_reverse(&comments); gal_table_write(p->objectcols, comments, p->cp.tableformat, p->objectsout, "OBJECTS"); gal_list_str_free(comments, 1); /* CLUMPS CATALOG ============== */ if(p->clumps) { comments=mkcatalog_outputs_same_start(p, 1, "Clumps"); /* Write objects catalog --------------------- Reverse the comments list (so it is printed in the same order here), write the objects catalog and free the comments. */ gal_list_str_reverse(&comments); gal_table_write(p->clumpcols, comments, p->cp.tableformat, p->clumpsout, "CLUMPS"); gal_list_str_free(comments, 1); } } /*********************************************************************/ /***************** Top-level function *******************/ /*********************************************************************/ void mkcatalog(struct mkcatalogparams *p) { /* When more than one thread is to be used, initialize the mutex: we need it to assign a column to the clumps in the final catalog. */ if( p->cp.numthreads > 1 ) pthread_mutex_init(&p->mutex, NULL); /* Do the processing on each thread. */ gal_threads_spin_off(mkcatalog_single_object, p, p->numobjects, p->cp.numthreads); /* Post-thread processing, for example to convert image coordinates to RA and Dec. */ mkcatalog_wcs_conversion(p); /* Write the filled columns into the output. */ mkcatalog_write_outputs(p); /* Destroy the mutex. */ if( p->cp.numthreads>1 ) pthread_mutex_destroy(&p->mutex); } ����������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/ui.c���������������������������������������������������������������������0000644�0001750�0001750�00000103503�13216276304�013442� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <inttypes.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro/arithmetic.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/tableintern.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "mkcatalog.h" #include "ui.h" #include "columns.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will create a catalog from " "an input, labeled, and noise images.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct mkcatalogparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_struct = p; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->poptions = program_options; cp->numthreads = gal_threads_number(); cp->coptions = gal_commonopts_options; /* Specific to this program. */ p->sfmagnsigma = NAN; p->sfmagarea = NAN; p->upnsigma = NAN; p->zeropoint = NAN; p->threshold = NAN; p->upsigmaclip[0] = NAN; p->upsigmaclip[1] = NAN; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: cp->coptions[i].flags=OPTION_HIDDEN; cp->coptions[i].mandatory=GAL_OPTIONS_NOT_MANDATORY; break; case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct mkcatalogparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->inputname) argp_error(state, "only one argument (input file) should be given"); else p->inputname=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /* Read the user's desired columns. Because the types of these options are `GAL_TYPE_INVALID', this function will not be called when printing the full list of parameters and their values. */ void * ui_column_codes_ll(struct argp_option *option, char *arg, char *filename, size_t lineno, void *params) { struct mkcatalogparams *p=(struct mkcatalogparams *)params; /* These options don't take arguments on the command-line but in the configuration files they can take values of 0 or 1. In the latter case, the column shouldn't be added if the value is 0. */ if(arg) { if( arg[0]=='0' && arg[1]=='\0' ) return NULL; else if ( !(arg[0]=='1' && arg[1]=='\0') ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' is not a " "valid value to the `%s' option: (\"%s\").\n\n`%s' is " "an on/off option specifying if you want this column " "in the output catalog, it doesn't take any " "arguments. In a configuration file, it can only take " "a value of `0' (to be ignored) or `1'", arg, option->name, option->doc, option->name); } /* The user wants this column, so add it to the list. Note that the `ids' column means three columns. */ if(option->key==UI_KEY_IDS) { gal_list_i32_add(&p->columnids, UI_KEY_OBJID); gal_list_i32_add(&p->columnids, UI_KEY_HOSTOBJID); gal_list_i32_add(&p->columnids, UI_KEY_IDINHOSTOBJ); } else gal_list_i32_add(&p->columnids, option->key); /* Return NULL */ return NULL; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. static void ui_read_check_only_options(struct mkcatalogparams *p) { } */ static void ui_check_options_and_arguments(struct mkcatalogparams *p) { /* Make sure an input file name was given and if it was a FITS file, that a HDU is also given. */ if(p->inputname) { if( gal_fits_name_is_fits(p->inputname) && p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified. When the input is a FITS " "file, a HDU must also be specified, you can use the `--hdu' " "(`-h') option and give it the HDU number (starting from " "zero), extension name, or anything acceptable by CFITSIO"); } else error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ /* If a WCS structure is present, then read its basic information to use in the table meta-data. */ static void ui_wcs_info(struct mkcatalogparams *p) { char *c; size_t i; /* Read the basic WCS information. */ if(p->input->wcs) { /* Allocate space for the array of strings. */ errno=0; p->ctype=malloc(p->input->ndim * sizeof *p->ctype); if(p->ctype==NULL) error(EXIT_FAILURE, 0, "%s: %zu bytes for `p->ctype'", __func__, p->input->ndim * sizeof *p->ctype); /* Fill in the values. */ for(i=0;i<p->input->ndim;++i) { /* CTYPE might contain `-' characters, we just want the first non-dash characters. The loop will either stop either at the end or where there is a dash. So we can just replace it with an end-of-string character. */ gal_checkset_allocate_copy(p->input->wcs->ctype[i], &p->ctype[i]); c=p->ctype[i]; while(*c!='\0' && *c!='-') ++c; *c='\0'; } } } static void ui_preparations_read_inputs(struct mkcatalogparams *p) { size_t one=1; int readclumps=0; char *namestypes, **strarr=NULL; gal_data_t *zero, *key=gal_data_array_calloc(1); char *skyfile=p->skyfile ? p->skyfile : p->inputname; char *stdfile=p->stdfile ? p->stdfile : p->inputname; char *clumpsfile=p->clumpsfile ? p->clumpsfile : p->inputname; char *objectsfile=p->objectsfile ? p->objectsfile : p->inputname; /* Read the input image. */ p->input=gal_fits_img_read_to_type(p->inputname, p->cp.hdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0,0); /* Read basic WCS information for final table meta-data. */ ui_wcs_info(p); /* Currently MakeCatalog is only implemented for 2D images. */ if(p->input->ndim!=2) error(EXIT_FAILURE, 0, "%s (hdu %s) has %zu dimensions, MakeCatalog " "currently only supports 2D inputs", p->inputname, p->cp.hdu, p->input->ndim); /* See if the input has blank pixels and set the flags appropriately. */ p->hasblank = gal_blank_present(p->input, 1); /* Read the object label image and check its size. */ p->objects = gal_fits_img_read(objectsfile, p->objectshdu, p->cp.minmapsize, 0, 0); if( gal_data_dsize_is_different(p->input, p->objects) ) error(EXIT_FAILURE, 0, "`%s' (hdu: %s) and `%s' (hdu: %s) have a" "different dimension/size", objectsfile, p->objectshdu, p->inputname, p->cp.hdu); /* Read the Sky image and check its size. */ p->sky=gal_fits_img_read_to_type(skyfile, p->skyhdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0, 0); if( gal_data_dsize_is_different(p->input, p->sky) ) error(EXIT_FAILURE, 0, "`%s' (hdu: %s) and `%s' (hdu: %s) have a" "different dimension/size", skyfile, p->skyhdu, p->inputname, p->cp.hdu); /* Read the Sky standard deviation image and check its size. */ p->std=gal_fits_img_read_to_type(stdfile, p->stdhdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0, 0); if( gal_data_dsize_is_different(p->input, p->std) ) error(EXIT_FAILURE, 0, "`%s' (hdu: %s) and `%s' (hdu: %s) have a" "different dimension/size", stdfile, p->stdhdu, p->inputname, p->cp.hdu); /* If an upper-limit mask image was given, read it. */ if(p->upmaskfile) { /* Read the mask image. */ p->upmask = gal_fits_img_read(p->upmaskfile, p->upmaskhdu, p->cp.minmapsize, 0, 0); if( gal_data_dsize_is_different(p->input, p->upmask) ) error(EXIT_FAILURE, 0, "`%s' (hdu: %s) and `%s' (hdu: %s) have a" "different dimension/size", p->upmaskfile, p->upmaskhdu, p->inputname, p->cp.hdu); /* If it isn't an integer type, report an error, otherwise, convert it to a uint8_t: with a 1 for all non-zero pixels and 0 for zero pixels. */ zero=gal_data_alloc(NULL, GAL_TYPE_UINT8, 1, &one, NULL, 1, -1, NULL, NULL, NULL); p->upmask=gal_arithmetic(GAL_ARITHMETIC_OP_NE, ( GAL_ARITHMETIC_INPLACE | GAL_ARITHMETIC_FREE | GAL_ARITHMETIC_NUMOK ), p->upmask, zero); } /* Check to see if the objects extension has a `WCLUMPS' keyword and that its value is 'yes', `y', or `1'. */ key->name="WCLUMPS"; key->type=GAL_TYPE_STRING; gal_fits_key_read(objectsfile, p->objectshdu, key, 0, 0); if(key->status==KEY_NO_EXIST) readclumps=0; else { if(key->status) gal_fits_io_error(key->status, "CFITSIO error while reading " "WCLUMPS keyword"); else { strarr=key->array; if( !strcasecmp(strarr[0], "yes") || !strcasecmp(strarr[0], "y") || !strcmp(strarr[0], "1") ) readclumps=1; } } /* Read the clumps array if necessary. */ if(readclumps) { /* Make sure the user did indeed give the clumps HDU. */ if(p->clumpshdu==NULL) error(EXIT_FAILURE, 0, "no `--clumpshdu' given! The WCLUMPS keyword " "in %s (hdu: %s) has a value of `%s', so MakeCatalog expects " "a clump image.\n\nYou can use the optional `--clumpsfile' " "option to give the filename and the mandatory `--clumpshdu' " "to specify the extension. If `--clumpsfile' is not given, " "MakeCatalog will look into the input file for the given " "extension. Alternatively, you can modify/remove this " "keyword using Gnuastro's Fits program, please run `$ info " "astfits' for more information (press `SPACE' to go down and " "`q' to return to the command-line).", objectsfile, p->objectshdu, strarr[0]); /* Read the clumps image and check its size. */ p->clumps = gal_fits_img_read(clumpsfile, p->clumpshdu, p->cp.minmapsize, 0, 0); if( gal_data_dsize_is_different(p->input, p->std) ) error(EXIT_FAILURE, 0, "`%s' (hdu: %s) and `%s' (hdu: %s) have a" "different dimension/size", clumpsfile, p->clumpshdu, p->inputname, p->cp.hdu); } /* Make sure the object and clump label images have an integer type, then to be safe that they have the correct integer type, run `gal_data_copy_to_new_type' on them. */ if( p->objects->type==GAL_TYPE_FLOAT32 || p->objects->type==GAL_TYPE_FLOAT64 || (p->clumps && ( p->clumps->type==GAL_TYPE_FLOAT32 || p->clumps->type==GAL_TYPE_FLOAT64 ) ) ) { if(p->clumps) asprintf(&namestypes, "However, `%s' (hdu: %s) and `%s' (hdu: %s) " "have types of `%s' and `%s' respectively", objectsfile, p->objectshdu, clumpsfile, p->clumpshdu, gal_type_name(p->objects->type, 1), gal_type_name(p->clumps->type, 1) ); else asprintf(&namestypes, "However, %s (hdu: %s) has a type of %s", objectsfile, p->objectshdu, gal_type_name(p->objects->type, 1)); error(EXIT_FAILURE, 0, "labeled images (for objects or clumps) must " "have an integer datatype. %s.\n\n" "If you are sure the images contain only integer values but " "are just stored in a floating point container, you can " "put them in an integer container with Gnuastro's Arithmetic " "program using a command like below:\n\n" " $ astarithmetic img.fits int32", namestypes); } p->objects=gal_data_copy_to_new_type_free(p->objects, GAL_TYPE_INT32); if(p->clumps) p->clumps=gal_data_copy_to_new_type_free(p->clumps, GAL_TYPE_INT32); /* Clean up. */ key->name=NULL; gal_data_array_free(key, 1, 1); } /* The input images can have extensions to speed up the processing. */ static void ui_preparations_read_keywords(struct mkcatalogparams *p) { char *msg; gal_data_t *tmp; gal_data_t *keys=gal_data_array_calloc(2); char *stdfile=p->stdfile ? p->stdfile : p->inputname; char *clumpsfile=p->clumpsfile ? p->clumpsfile : p->inputname; char *objectsfile=p->objectsfile ? p->objectsfile : p->inputname; /* Read the keywords from the standard deviation image. */ keys[0].next=&keys[1]; keys[0].name="MINSTD"; keys[1].name="MEDSTD"; keys[0].type=GAL_TYPE_FLOAT32; keys[1].type=GAL_TYPE_FLOAT32; keys[0].array=&p->minstd; keys[1].array=&p->medstd; gal_fits_key_read(stdfile, p->stdhdu, keys, 0, 0); /* If the two keywords couldn't be read, calculate them. */ if(keys[0].status) { /* Calculate the minimum STD. */ tmp=gal_statistics_minimum(p->std); p->minstd=*((float *)(tmp->array)); gal_data_free(tmp); } if(keys[1].status) { /* Calculate the median STD. */ tmp=gal_statistics_median(p->std, 0); p->medstd=*((float *)(tmp->array)); gal_data_free(tmp); /* Alert the user if it wasn't calculated from a header keyword. */ fprintf(stderr, "---------------\n" "Warning: Could not find the `MEDSTD' keyword in `%s' " "(hdu: %s). The median standard deviation is thus found on " "the (interpolated) standard deviation image. NoiseChisel " "finds the median before interpolation which is more " "accurate. Ho the reported value in the final catalog will " "not be accurate: it will depend on how many tiles were " "blank and their spatial position relative to the non-blank " "ones.\n" "---------------\n", stdfile, p->stdhdu); } p->cpscorr = p->minstd>1 ? 1.0f : p->minstd; /* Read the keywords from the objects image. */ keys[0].name="DETSN"; keys[1].name="NUMLABS"; keys[0].type=GAL_TYPE_FLOAT32; keys[1].type=GAL_TYPE_SIZE_T; keys[0].array=&p->detsn; keys[1].array=&p->numobjects; gal_fits_key_read(objectsfile, p->objectshdu, keys, 0, 0); if(keys[0].status) p->detsn=NAN; /* When `status!=0', then */ if(keys[1].status) /* the key couldn't be read. */ { tmp=gal_statistics_maximum(p->objects); p->numobjects=*((int32_t *)(tmp->array)); /*numobjects is in int32_t.*/ gal_data_free(tmp); } /* If there were no objects in the input, then inform the user with an error (no catalog was built). */ if(p->numobjects==0) error(EXIT_FAILURE, 0, "no object labels (non-zero pixels) in " "%s (hdu %s). To make a catalog, labeled regions must be defined", objectsfile, p->objectshdu); /* Read the keywords from the clumps image if necessary. */ if(p->clumps) { keys[0].name="CLUMPSN"; keys[1].name="NUMLABS"; keys[0].type=GAL_TYPE_FLOAT32; keys[1].type=GAL_TYPE_SIZE_T; keys[0].array=&p->clumpsn; keys[1].array=&p->numclumps; gal_fits_key_read(clumpsfile, p->clumpshdu, keys, 0, 0); if(keys[0].status) p->clumpsn=NAN; if(keys[1].status) { asprintf(&msg, "couldn't find/read NUMLABS in the header of " "%s (hdu: %s), see error above", clumpsfile, p->clumpshdu); gal_fits_io_error(keys[1].status, msg); } } /* If there were no clumps, then free the clumps array and set it to NULL, so for the rest of the processing, MakeCatalog things that no clumps image was given. */ if(p->numclumps==0) { gal_data_free(p->clumps); p->clumps=NULL; } /* Clean up. */ keys[0].name=keys[1].name=NULL; keys[0].array=keys[1].array=NULL; gal_data_array_free(keys, 2, 1); } /* To make the catalog processing more scalable (and later allow for over-lappping regions), we will define a tile for each object. */ void ui_one_tile_per_object(struct mkcatalogparams *p) { size_t ndim=p->input->ndim; int32_t *l, *lf, *start; size_t i, d, *min, *max, width=2*ndim; size_t *minmax=gal_data_malloc_array(GAL_TYPE_SIZE_T, width*p->numobjects, __func__, "minmax"); size_t *coord=gal_data_malloc_array(GAL_TYPE_SIZE_T, ndim, __func__, "coord"); /* Initialize the minimum and maximum position for each tile/object. So, we'll initialize the minimum coordinates to the maximum possible `size_t' value (in `GAL_BLANK_SIZE_T') and the maximums to zero. */ for(i=0;i<p->numobjects;++i) for(d=0;d<ndim;++d) { minmax[ i * width + d ] = GAL_BLANK_SIZE_T; /* Minimum. */ minmax[ i * width + ndim + d ] = 0; /* Maximum. */ } /* Go over the objects label image and correct the minimum and maximum coordinates. */ start=p->objects->array; lf=(l=p->objects->array)+p->objects->size; do if(*l>0) { /* Get the coordinates of this pixel. */ gal_dimension_index_to_coord(l-start, ndim, p->objects->dsize, coord); /* Check to see this coordinate is the smallest/largest found so far for this label. Note that labels start from 1, while indexs here start from zero. */ min = &minmax[ (*l-1) * width ]; max = &minmax[ (*l-1) * width + ndim ]; for(d=0;d<ndim;++d) { if( coord[d] < min[d] ) min[d] = coord[d]; if( coord[d] > max[d] ) max[d] = coord[d]; } } while(++l<lf); /* For a check. for(i=0;i<p->numobjects;++i) printf("%zu: (%zu, %zu) --> (%zu, %zu)\n", i+1, minmax[i*width], minmax[i*width+1], minmax[i*width+2], minmax[i*width+3]); */ /* Make the tiles. */ p->tiles=gal_tile_series_from_minmax(p->input, minmax, p->numobjects); /* Clean up. */ free(coord); free(minmax); } /* When both catalogs need to be made, we need a separator, the output names will either be built based on the input name or output name (if given). In both cases, the operations are the same, just the base name differs. So to keep things clean, we have defined this function. */ static void ui_preparations_both_names(struct mkcatalogparams *p) { char *basename, *suffix=".fits"; uint8_t keepinputdir=p->cp.keepinputdir; /* See below. */ /* Set the type ending. */ if(p->cp.output) { /* When the user has specified a name, any possible directories in that name must be respected. So we have kept the actual `keepinputdir' value in a temporary variable above and set it to 1 only for this operation. Later we set it back to what it was. */ p->cp.keepinputdir=1; /* Set the base name (if necessary). */ basename = p->cp.output; /* FITS speicifc preparations. */ if( gal_fits_name_is_fits(p->cp.output) ) { /* The output file name that the user has given supersedes the `tableformat' argument. In this case, the filename is a FITS file, so if `tableformat' is a text file, we will change it to a default binary FITS table. */ if( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ) p->cp.tableformat=GAL_TABLE_FORMAT_BFITS; } } else { /* Note that suffix is not used in the text table outputs, so it doesn't matter if the output table is not FITS. */ suffix="_catalog.fits"; basename = p->inputname; } /* Set the final filename. If the output is a text file, we need two files. But when its a FITS file we want to make a multi-extension FITS file. */ if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) { p->objectsout=gal_checkset_automatic_output(&p->cp, basename, "_o.txt"); p->clumpsout=gal_checkset_automatic_output(&p->cp, basename, "_c.txt"); } else { p->objectsout=gal_checkset_automatic_output(&p->cp, basename, suffix); p->clumpsout=p->objectsout; } /* Revert `keepinputdir' to what it was and free `p->cp.output', we will be using `p->objectsout' and `p->clumpsout' from now on. */ if(p->cp.output) { p->cp.keepinputdir=keepinputdir; free(p->cp.output); p->cp.output=NULL; } } /* Set the output name. */ static void ui_preparations_outnames(struct mkcatalogparams *p) { char *suffix; /* Set the output filename */ if(p->cp.output) { /* If the output name is a FITS file, then `gal_tableintern_check_fits_format' will see if the tableformat corresponds to a FITS table or not. If the output name isn't a FITS file then the current value of `p->cp.tableformat' is irrelevant and it must be set to text. We use this value in the end to determine specific features. */ if( gal_fits_name_is_fits(p->cp.output) ) gal_tableintern_check_fits_format(p->cp.output, p->cp.tableformat); else p->cp.tableformat=GAL_TABLE_FORMAT_TXT; /* If a clumps image has been read, then we have two outputs. */ if(p->clumps) ui_preparations_both_names(p); else { gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); p->objectsout=p->cp.output; p->cp.output=NULL; } } else { /* Both clumps and object catalogs are necessary. */ if(p->clumps) ui_preparations_both_names(p); /* We only need one objects catalog. */ else { suffix = ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "._cat.txt" : "_cat.fits" ); p->objectsout=gal_checkset_automatic_output(&p->cp, p->inputname, suffix); } } } /* Sanity checks and preparations for the upper-limit magnitude. */ static void ui_preparations_upperlimit(struct mkcatalogparams *p) { size_t i, c=0; /* Check if the given range has the same number of elements as dimensions in the input. */ if(p->uprange) { for(i=0;p->uprange[i]!=-1;++i) ++c; if(c!=p->input->ndim) error(EXIT_FAILURE, 0, "%zu values given to `--uprange', but input " "has %zu dimensions", c, p->input->ndim); } /* Check the number of random samples. */ if( p->upnum < MKCATALOG_UPPERLIMIT_MINIMUM_NUM ) error(EXIT_FAILURE, 0, "%zu not acceptable as `--upnum'. The minimum " "acceptable number of random samples for the upper limit " "magnitude is %d", p->upnum, MKCATALOG_UPPERLIMIT_MINIMUM_NUM); /* Check if sigma-clipping parameters have been given. */ if( isnan(p->upsigmaclip[0]) ) error(EXIT_FAILURE, 0, "`--upsigmaclip' is mandatory for measuring " "the upper-limit magnitude. It takes two numbers separated by " "a comma. The first is the multiple of sigma and the second is " "the aborting criteria: <1: tolerance level, >1: number of " "clips"); /* Check if the sigma multiple is given. */ if( isnan(p->upnsigma) ) error(EXIT_FAILURE, 0, "`--upnsigma' is mandatory for measuring the " "upperlimit magnitude. Its value is the multiple of final sigma " "that is reported as the upper-limit"); /* Set the random number generator. */ gsl_rng_env_setup(); p->rng=gsl_rng_alloc(gsl_rng_ranlxs1); p->seed = ( p->envseed ? gsl_rng_default_seed : gal_timing_time_based_rng_seed() ); if(p->envseed) gsl_rng_set(p->rng, p->seed); p->rngname=gsl_rng_name(p->rng); /* Keep the minimum and maximum values of the random number generator. */ p->rngmin=gsl_rng_min(p->rng); p->rngdiff=gsl_rng_max(p->rng)-p->rngmin; } void ui_preparations(struct mkcatalogparams *p) { /* If no columns are requested, then inform the user. */ if(p->columnids==NULL) error(EXIT_FAILURE, 0, "no columns requested, please run again with " "`--help' for the full list of columns you can ask for"); /* Read the inputs. */ ui_preparations_read_inputs(p); /* Read the helper keywords from the inputs and if they aren't present then calculate the necessary parameters. */ ui_preparations_read_keywords(p); /* Set the output filename(s). */ ui_preparations_outnames(p); /* Allocate the output columns to fill up with the program. */ columns_define_alloc(p); /* Make the tiles that cover each object. */ ui_one_tile_per_object(p); /* Allocate the reference random number generator and seed values. It will be cloned once for every thread. If the user hasn't called `envseed', then we want it to be different for every run, so we need to re-set the seed. */ if(p->upperlimit) ui_preparations_upperlimit(p); if( p->hasmag && isnan(p->zeropoint) ) error(EXIT_FAILURE, 0, "no zeropoint specified"); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct mkcatalogparams *p) { struct gal_options_common_params *cp=&p->cp; char *skyfile, *stdfile, *clumpsfile, *objectsfile; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. ui_read_check_only_options(p); */ /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Inform the user. */ if(!p->cp.quiet) { /* Set the names for easy reading. */ skyfile = p->skyfile ? p->skyfile : p->inputname; stdfile = p->stdfile ? p->stdfile : p->inputname; clumpsfile = p->clumpsfile ? p->clumpsfile : p->inputname; objectsfile = p->objectsfile ? p->objectsfile : p->inputname; /* Write the information. */ printf(PROGRAM_NAME" started on %s", ctime(&p->rawtime)); printf(" - Using %zu CPU thread%s\n", p->cp.numthreads, p->cp.numthreads==1 ? "." : "s."); printf(" - Input: %s (hdu: %s)\n", p->inputname, p->cp.hdu); printf(" - Objects: %s (hdu: %s)\n", objectsfile, p->objectshdu); if(p->clumps) printf(" - Clumps: %s (hdu: %s)\n", clumpsfile, p->clumpshdu); printf(" - Sky: %s (hdu: %s)\n", skyfile, p->skyhdu); printf(" - Sky STD: %s (hdu: %s)\n", stdfile, p->stdhdu); if(p->upmaskfile) printf(" - Upper limit magnitude mask: %s (hdu: %s)\n", p->upmaskfile, p->cp.hdu); if(p->upperlimit) { printf(" - Random number generator name: %s\n", p->rngname); printf(" - Random number generator seed: %"PRIu64"\n", p->seed); } } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct mkcatalogparams *p, struct timeval *t1) { size_t d; /* The temporary arrays for WCS coordinates. */ if(p->wcs_vo ) gal_list_data_free(p->wcs_vo); if(p->wcs_vc ) gal_list_data_free(p->wcs_vc); if(p->wcs_go ) gal_list_data_free(p->wcs_go); if(p->wcs_gc ) gal_list_data_free(p->wcs_gc); if(p->wcs_vcc) gal_list_data_free(p->wcs_vcc); if(p->wcs_gcc) gal_list_data_free(p->wcs_gcc); /* Free the types of the WCS coordinates (for catalog meta-data). */ if(p->ctype) { for(d=0;d<p->input->ndim;++d) free(p->ctype[d]); free(p->ctype); } /* If a random number generator was allocated, free it. */ if(p->rng) gsl_rng_free(p->rng); /* Free output names. */ if(p->clumpsout && p->clumpsout!=p->objectsout) free(p->clumpsout); free(p->objectsout); /* Free the allocated arrays: */ free(p->skyhdu); free(p->stdhdu); free(p->cp.hdu); free(p->oiflag); free(p->ciflag); free(p->skyfile); free(p->stdfile); free(p->clumpshdu); free(p->objectshdu); free(p->clumpsfile); free(p->objectsfile); gal_data_free(p->sky); gal_data_free(p->std); gal_data_free(p->input); gal_data_free(p->upmask); gal_data_free(p->clumps); gal_data_free(p->objects); gal_data_array_free(p->tiles, p->numobjects, 0); /* Print the final message. */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/main.c�������������������������������������������������������������������0000644�0001750�0001750�00000003230�13121462410�013733� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* MakeCatalog - Make a catalog from an input and labeled image. MakeCatalog is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" /* needs main.h. */ #include "mkcatalog.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct mkcatalogparams p={{{0},0},0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ mkcatalog(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/Makefile.in��������������������������������������������������������������0000644�0001750�0001750�00000211767�13217217705�014743� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software 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= @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for MakeCatalog. # MakeCatalog is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astmkcatalog --help # Full list of options, short doc. # $ astmkcatalog -P # Print all options and used values. # $ info astmkcatalog # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Input: hdu 1 objectshdu 2 clumpshdu 3 skyhdu SKY stdhdu SKY_STD zeropoint 0.0 skysubtracted 0 # Output: sfmagnsigma 1 sfmagarea 1 # Upper limit magnitude: upnum 100 upsigmaclip 3,0.2 upnsigma 1 # Catalog columns: ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/mkcatalog/Makefile.am��������������������������������������������������������������0000644�0001750�0001750�00000002672�13121462410�014710� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astmkcatalog astmkcatalog_LDADD = -lgnuastro astmkcatalog_SOURCES = main.c ui.c mkcatalog.c columns.c upperlimit.c EXTRA_DIST = main.h authors-cite.h args.h ui.h mkcatalog.h columns.h \ upperlimit.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmkcatalog.conf ����������������������������������������������������������������������gnuastro-0.5/bin/match/�����������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�012070� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/match.h����������������������������������������������������������������������0000644�0001750�0001750�00000002051�13211076737�013257� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MATCH_H #define MATCH_H void match(struct matchparams *p); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/ui.h�������������������������������������������������������������������������0000644�0001750�0001750�00000003470�13211616535�012602� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Group codes. */ enum program_args_groups { UI_GROUP_CATALOGMATCH = GAL_OPTIONS_GROUP_AFTER_COMMON, }; /* Available letters for short options: b d e f g i j k m n p r s t u v w x y z A B E G J L O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_HDU2 = 'H', UI_KEY_APERTURE = 'a', UI_KEY_LOGASOUTPUT = 'l', UI_KEY_CCOL1 = 'c', UI_KEY_CCOL2 = 'C', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_NOTMATCHED = 1000, UI_KEY_OUTCOLS, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct matchparams *p); void ui_free_report(struct matchparams *p, struct timeval *t1); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/args.h�����������������������������������������������������������������������0000644�0001750�0001750�00000007777�13216276304�013140� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { /* Input file parameters. */ { "hdu2", UI_KEY_HDU2, "STR/INT", 0, "Extension name or number of second input.", GAL_OPTIONS_GROUP_INPUT, &p->hdu2, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Outputs. */ { "logasoutput", UI_KEY_LOGASOUTPUT, 0, 0, "No rearranging of inputs, output is log file", GAL_OPTIONS_GROUP_OUTPUT, &p->logasoutput, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "notmatched", UI_KEY_NOTMATCHED, 0, 0, "Output is rows that don't match.", GAL_OPTIONS_GROUP_OUTPUT, &p->notmatched, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "outcols", UI_KEY_OUTCOLS, "STR", 0, "Out cols in CSV, `a': first, `b': second input.", GAL_OPTIONS_GROUP_OUTPUT, &p->outcols, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_strings }, /* Catalog matching. */ { 0, 0, 0, 0, "Catalog matching", UI_GROUP_CATALOGMATCH }, { "ccol1", UI_KEY_CCOL1, "STR[,STR]", 0, "Column name/number of first catalog.", UI_GROUP_CATALOGMATCH, &p->ccol1, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_strings }, { "ccol2", UI_KEY_CCOL2, "STR[,STR]", 0, "Column name/number of second catalog.", UI_GROUP_CATALOGMATCH, &p->ccol2, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_strings }, { "aperture", UI_KEY_APERTURE, "FLT[,FLT[,FLT]]", 0, "Acceptable aperture for matching.", UI_GROUP_CATALOGMATCH, &p->aperture, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, {0} }; /* Define the child argp structure ------------------------------- NOTE: these parts can be left untouched.*/ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif �gnuastro-0.5/bin/match/authors-cite.h���������������������������������������������������������������0000644�0001750�0001750�00000002764�13211076737�014605� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ������������gnuastro-0.5/bin/match/main.h�����������������������������������������������������������������������0000644�0001750�0001750�00000005723�13211616535�013114� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "Match" /* Program full name. */ #define PROGRAM_EXEC "astmatch" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION enum match_modes { MATCH_MODE_INVALID, /* ==0 by default. */ MATCH_MODE_WCS, MATCH_MODE_CATALOG, }; /* Main program parameters structure */ struct matchparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ char *input1name; /* First input filename. */ char *input2name; /* Second input filename. */ char *hdu2; /* Second input's HDU. */ gal_data_t *ccol1; /* Array of firs input column names. */ gal_data_t *ccol2; /* Array of second input column names. */ gal_data_t *outcols; /* Array of second input column names. */ gal_data_t *aperture; /* Acceptable matching aperture. */ uint8_t logasoutput; /* Don't rearrange inputs, out is log. */ uint8_t notmatched; /* Output is rows that don't match. */ /* Internal */ int mode; /* Mode of operation: image or catalog. */ gal_data_t *cols1; /* Column values of first input. */ gal_data_t *cols2; /* Column values of second input. */ gal_list_str_t *acols; /* Output columns from first input. */ gal_list_str_t *bcols; /* Output columns from second input. */ char *logname; /* Name of log file. */ char *out1name; /* Name of first matched output. */ char *out2name; /* Name of second matched output. */ /* Output: */ time_t rawtime; /* Starting time of the program. */ }; #endif ���������������������������������������������gnuastro-0.5/bin/match/match.c����������������������������������������������������������������������0000644�0001750�0001750�00000022466�13211616535�013262� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <gnuastro/match.h> #include <gnuastro/table.h> #include <gnuastro/permutation.h> #include <gnuastro-internal/checkset.h> #include <main.h> /* Read the catalog in the given file and use the given permutation to keep the proper columns. */ static gal_data_t * match_catalog_read_write_all(struct matchparams *p, size_t *permutation, size_t nummatched, int f1s2, size_t **numcolmatch) { size_t origsize; gal_data_t *tmp, *cat; gal_list_void_t *arrays=NULL; char *hdu = (f1s2==1) ? p->cp.hdu : p->hdu2; gal_list_str_t *cols = (f1s2==1) ? p->acols : p->bcols; char *extname = (f1s2==1) ? "INPUT_1" : "INPUT_2"; char *outname = (f1s2==1) ? p->out1name : p->out2name; char *filename = (f1s2==1) ? p->input1name : p->input2name; /* When the output contains columns from both inputs, we need to keep the number of columns matched against each column identifier. */ if(p->outcols) *numcolmatch=gal_data_malloc_array(GAL_TYPE_SIZE_T, gal_list_str_number(cols), __func__, "numcolmatch"); /* Read the full table. */ cat=gal_table_read(filename, hdu, cols, p->cp.searchin, p->cp.ignorecase, p->cp.minmapsize, *numcolmatch); origsize=cat->size; /* Go over each column and permute its contents. */ for(tmp=cat; tmp!=NULL; tmp=tmp->next) { /* Do the permutation. */ gal_permutation_apply(tmp, permutation); /* Correct the size of the array so only the matching columns are saved as output. This is only Gnuastro's convention, it has no effect on later freeing of the array in the memory. */ if(p->notmatched) { /* Add the original array pointer to a list (we need to reset it later). */ gal_list_void_add(&arrays, tmp->array); /* Reset the data structure's array element to start where the non-matched elements start. */ tmp->array=gal_data_ptr_increment(tmp->array, nummatched, tmp->type); /* Correct the size of the tile. */ tmp->size = tmp->dsize[0] = tmp->size - nummatched; } else tmp->size=tmp->dsize[0]=nummatched; } /* Write the catalog to the output. */ if(p->outcols) return cat; else { /* Write the catalog to a file. */ gal_table_write(cat, NULL, p->cp.tableformat, outname, extname); /* Correct arrays and sizes (when `notmatched' was called). The `array' element has to be corrected for later freeing. IMPORTANT: `--notmatched' cannot be called with `--outcols'. So you don't have to worry about the checks here being done later. */ if(p->notmatched) { /* Reverse the list of array pointers to write them back in. */ gal_list_void_reverse(&arrays); /* Correct the array and size pointers. */ for(tmp=cat; tmp!=NULL; tmp=tmp->next) { tmp->array=gal_list_void_pop(&arrays); tmp->size=tmp->dsize[0]=origsize; tmp->block=NULL; } } /* Clean up. */ gal_list_data_free(cat); return NULL; } } /* When specific columns from both inputs are requested, this function will write them out into a single table. */ static void match_catalog_write_one(struct matchparams *p, gal_data_t *a, gal_data_t *b, size_t *acolmatch, size_t *bcolmatch) { gal_data_t *cat=NULL; size_t i, j, ac=0, bc=0; char **strarr=p->outcols->array; /* Go over the initial list of strings. */ for(i=0; i<p->outcols->size; ++i) switch(strarr[i][0]) { case 'a': for(j=0;j<acolmatch[ac];++j) gal_list_data_add(&cat, gal_list_data_pop(&a)); ac++; break; case 'b': for(j=0;j<bcolmatch[bc];++j) gal_list_data_add(&cat, gal_list_data_pop(&b)); bc++; break; default: error(EXIT_FAILURE, 0, "a bug! Please contact us at %s to fix the " "problem. the value to strarr[%zu][0] (%c) is not recognized", PACKAGE_BUGREPORT, i, strarr[i][0]); } /* Reverse the table and write it out. */ gal_list_data_reverse(&cat); gal_table_write(cat, NULL, p->cp.tableformat, p->cp.output, "MATCHED"); } static void match_catalog(struct matchparams *p) { uint32_t *u, *uf; gal_data_t *tmp, *mcols; gal_data_t *a=NULL, *b=NULL; size_t nummatched, *acolmatch, *bcolmatch; /* Find the matching coordinates. We are doing the processing in place, */ mcols=gal_match_coordinates(p->cols1, p->cols2, p->aperture->array, 0, 1, p->cp.minmapsize, &nummatched); /* If a match was found, then make the output files. */ if(mcols) { /* Read all the first catalog columns. */ if(p->logasoutput==0) { /* Read (and possibly write) the outputs. Note that we only need to read the table when it is necessary for the output (the user user might have asked for `--outcols', only with columns of one of the two inputs. */ if(p->outcols==NULL || p->acols) a=match_catalog_read_write_all(p, mcols->array, nummatched, 1, &acolmatch); if(p->outcols==NULL || p->bcols) b=match_catalog_read_write_all(p, mcols->next->array, nummatched, 2, &bcolmatch); /* If one catalog (with specific columns from either of the two inputs) was requested, then write it out. */ if(p->outcols) { /* Arrange the columns and write the output. */ match_catalog_write_one(p, a, b, acolmatch, bcolmatch); /* Clean up. */ if(acolmatch) free(acolmatch); if(bcolmatch) free(bcolmatch); } } /* Write the raw information in a log file if necessary. */ if(p->logname) { /* Note that unsigned 64-bit integers are not recognized in FITS tables. So if the log file is a FITS table, covert the two index columns to uint32. */ tmp=gal_data_copy_to_new_type(mcols, GAL_TYPE_UINT32); tmp->next=mcols->next; tmp->size=nummatched; gal_data_free(mcols); mcols=tmp; /* We also want everything to be incremented by one. In a C program, counting starts with zero, so `gal_match_coordinates' will return indexs starting from zero. But outside a C program, on the command-line people expect counting to start from 1 (for example with AWK). */ uf = (u=mcols->array) + tmp->size; do (*u)++; while(++u<uf); /* Same for the second set of indexs. */ tmp=gal_data_copy_to_new_type(mcols->next, GAL_TYPE_UINT32); uf = (u=tmp->array) + tmp->size; do (*u)++; while(++u<uf); tmp->next=mcols->next->next; gal_data_free(mcols->next); tmp->size=nummatched; mcols->next=tmp; /* Correct the comments. */ free(mcols->comment); mcols->comment="Row index in first catalog (counting from 1)."; free(mcols->next->comment); mcols->next->comment="Row index in second catalog (counting " "from 1)."; /* Write them into the table. */ gal_table_write(mcols, NULL, p->cp.tableformat, p->logname, "LOG_INFO"); /* Set the comment pointer to NULL: they weren't allocated. */ mcols->comment=NULL; mcols->next->comment=NULL; } gal_list_data_free(mcols); } /* Print the number of matches if not in quiet mode. */ if(!p->cp.quiet) fprintf(stdout, "%zu\n", nummatched); } /*******************************************************************/ /************* Top level function *************/ /*******************************************************************/ void match(struct matchparams *p) { if(p->mode==MATCH_MODE_CATALOG) match_catalog(p); } ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/ui.c�������������������������������������������������������������������������0000644�0001750�0001750�00000054355�13216276304�012606� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <gnuastro/fits.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" matches catalogs of objects " "and (by default) will return the re-arranged matching inputs. The " "optional log file will return low-level information about the match " "(indexs and distances).\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct matchparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: cp->coptions[i].doc="Extension name or number of first input."; break; case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_NUMTHREADS: cp->coptions[i].flags=OPTION_HIDDEN; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct matchparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->input1name) { if(p->input2name) argp_error(state, "only two arguments (input files) should be " "given"); else p->input2name=arg; } else p->input1name=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct matchparams *p) { if(p->outcols && p->notmatched) error(EXIT_FAILURE, 0, "`--outcols' and `--notmatched' cannot be called " "at the same time. The former is only for cases when the matches " "are required"); } static void ui_check_options_and_arguments(struct matchparams *p) { /* Make sure two input file names were given and if they a FITS file, that a HDU is also given for each. */ if(p->input1name) { if( gal_fits_name_is_fits(p->input1name) && p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU for first input. When the input is " "a FITS file, a HDU must also be specified, you can use the " "`--hdu' (`-h') option and give it the HDU number (starting " "from zero), extension name, or anything acceptable by " "CFITSIO"); } else error(EXIT_FAILURE, 0, "no input file is specified: two inputs are " "necessary"); if(p->input2name) { if( gal_fits_name_is_fits(p->input2name) && p->hdu2==NULL ) error(EXIT_FAILURE, 0, "no HDU for second input. Please use the " "`--hdu2' (`-H') option and give it the HDU number (starting " "from zero), extension name, or anything acceptable by " "CFITSIO"); } else error(EXIT_FAILURE, 0, "second input file not specified: two inputs are " "necessary"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ static void ui_set_mode(struct matchparams *p) { /* Check if we are in image or catalog mode. We will base the mode on the first input, then check with the second. */ if( gal_fits_name_is_fits(p->input1name) ) p->mode = ( (gal_fits_hdu_format(p->input1name, p->cp.hdu) == IMAGE_HDU) ? MATCH_MODE_WCS : MATCH_MODE_CATALOG ); else p->mode=MATCH_MODE_CATALOG; /* Now that the mode is set, check the second input's type. */ if( gal_fits_name_is_fits(p->input2name) ) { if(gal_fits_hdu_format(p->input2name, p->hdu2) == IMAGE_HDU) { if( p->mode==MATCH_MODE_CATALOG) error(EXIT_FAILURE, 0, "%s is a catalog, while %s is an image. " "Both inputs have to be images or catalogs", gal_checkset_dataset_name(p->input1name, p->cp.hdu), gal_checkset_dataset_name(p->input2name, p->hdu2) ); } else { if( p->mode==MATCH_MODE_WCS) error(EXIT_FAILURE, 0, "%s is an image, while %s is a catalog. " "Both inputs have to be images or catalogs", gal_checkset_dataset_name(p->input1name, p->cp.hdu), gal_checkset_dataset_name(p->input2name, p->hdu2)); } } else if(p->mode==MATCH_MODE_WCS) error(EXIT_FAILURE, 0, "%s is an image, while %s is a catalog! Both " "inputs have to be images or catalogs", gal_checkset_dataset_name(p->input1name, p->cp.hdu), gal_checkset_dataset_name(p->input2name, p->hdu2)); } /* The final aperture must have the following values: p->aperture[0]: Major axis length. p->aperture[1]: Axis ratio. p->aperture[2]: Position angle (relative to first dim). */ static void ui_read_columns_aperture_2d(struct matchparams *p) { size_t apersize=3; gal_data_t *newaper=NULL; double *naper, *oaper=p->aperture->array; /* A general sanity check: the first two elements of aperture cannot be zero or negative. */ if( oaper[0]<=0 ) error(EXIT_FAILURE, 0, "the first value of `--aperture' cannot be " "zero or negative"); if( p->aperture->size>1 && oaper[1]<=0 ) error(EXIT_FAILURE, 0, "the second value of `--aperture' cannot be " "zero or negative"); /* Will be needed in more than one case. */ if(p->aperture->size!=3) { newaper=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 1, &apersize, NULL, 0, -1, NULL, NULL, NULL); naper=newaper->array; } /* Different based on */ switch(p->aperture->size) { case 1: naper[0]=oaper[0]; naper[1]=1; naper[2]=0; break; case 2: naper[0] = oaper[0]>oaper[1] ? oaper[0] : oaper[1]; naper[1] = oaper[0]>oaper[1] ? oaper[1]/oaper[0] : oaper[0]/oaper[1]; naper[2] = oaper[0]>oaper[1] ? 0 : 90; break; case 3: if(oaper[1]>1) error(EXIT_FAILURE, 0, "second value to `--aperture' is larger " "than one. When three numbers are given to this option, the " "second is the axis ratio (which must always be less than 1)."); break; default: error(EXIT_FAILURE, 0, "%zu values given to `--aperture'. In 2D, this " "option can only take 1, 2, or 3 values", p->aperture->size); } /* If a new aperture was defined, then replace it with the exitsting one. */ if(newaper) { gal_data_free(p->aperture); p->aperture=newaper; } } /* We want to keep the columns as double type. So what-ever their original type is, convert it. */ static gal_data_t * ui_read_columns_to_double(struct matchparams *p, char *filename, char *hdu, gal_list_str_t *cols, size_t numcols) { gal_data_t *tmp, *ttmp, *tout, *out=NULL; struct gal_options_common_params *cp=&p->cp; char *diff_cols_error="%s: the number of columns matched (%zu) " "differs from the number of usable calls to `--ccol1' (%zu). " "Please give more specific values to `--ccol1' (column " "numberes are the only identifiers guaranteed to be unique)."; /* Read the columns. */ tout=gal_table_read(filename, hdu, cols, cp->searchin, cp->ignorecase, cp->minmapsize, NULL); /* A small sanity check. */ if(gal_list_data_number(tout)!=numcols) error(EXIT_FAILURE, 0, diff_cols_error, gal_checkset_dataset_name(filename, hdu), gal_list_data_number(tout), numcols); /* Go over the columns and see if they are double or not. To keep things simple, we'll keep a new list even if all the types are float64.*/ tmp=tout; while(tmp!=NULL) { /* We need ot set the `next' pointer */ ttmp=tmp->next; tmp->next=NULL; /* Correct the type if necessary. */ if(tmp->type==GAL_TYPE_FLOAT64) gal_list_data_add(&out, tmp); else gal_list_data_add(&out, gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT64) ); /* Set `tmp' to the initial `next pointer. */ tmp=ttmp; } /* The `out' above is in reverse, so correct it and return */ gal_list_data_reverse(&out); return out; } /* Read catalog columns */ static void ui_read_columns(struct matchparams *p) { size_t i; size_t ccol1n=p->ccol1->size; size_t ccol2n=p->ccol2->size; gal_list_str_t *cols1=NULL, *cols2=NULL; char **strarr1=p->ccol1->array, **strarr2=p->ccol2->array; /* Make sure the same number of columns is given to both. */ if(ccol1n!=ccol2n) error(EXIT_FAILURE, 0, "the number of values given to `--ccol1' and " "`--ccol2' (%zu and %zu) are not equal", ccol1n, ccol2n); /* Read/check the aperture values. */ if(p->aperture) switch(ccol1n) { case 1: if(p->aperture->size>1) error(EXIT_FAILURE, 0, "%zu values given to `--aperture'. In a 1D " "match, this option can only take one value", p->aperture->size); break; case 2: ui_read_columns_aperture_2d(p); break; default: error(EXIT_FAILURE, 0, "%zu dimensional matches are not currently " "supported (maximum is 2 dimensions). The number of " "dimensions is deduced from the number of values given to " "`--ccol1' and `--ccol2'", ccol1n); } else error(EXIT_FAILURE, 0, "no matching aperture specified. Please use " "the `--aperture' option to define the acceptable aperture for " "matching the coordinates (in the same units as each " "dimension). Please run the following command for more " "information.\n\n $ info %s\n", PROGRAM_EXEC); /* Convert the array of strings to a list of strings for the column names. */ for(i=0;i<ccol1n;++i) { gal_list_str_add(&cols1, strarr1[i], 0); gal_list_str_add(&cols2, strarr2[i], 0); strarr1[i]=strarr2[i]=NULL; /* So they are not freed later. */ } gal_list_str_reverse(&cols1); gal_list_str_reverse(&cols2); /* Read the columns. */ if(p->cp.searchin) { /* Read the first dataset. */ p->cols1=ui_read_columns_to_double(p, p->input1name, p->cp.hdu, cols1, ccol1n); p->cols2=ui_read_columns_to_double(p, p->input2name, p->hdu2, cols2, ccol2n); } else error(EXIT_FAILURE, 0, "no `--searchin' option specified. Please run " "the following command for more information:\n\n" " $ info gnuastro \"selecting table columns\"\n"); /* Free the extra spaces. */ gal_list_str_free(cols1, 1); gal_list_str_free(cols2, 1); gal_data_free(p->ccol1); gal_data_free(p->ccol2); p->ccol1=p->ccol2=NULL; } static void ui_preparations_out_cols(struct matchparams *p) { size_t i; char **strarr=p->outcols->array; /* Go over all the values and put the respective column identifier in the proper list. */ for(i=0;i<p->outcols->size;++i) switch(strarr[i][0]) { case 'a': gal_list_str_add(&p->acols, strarr[i]+1, 0); break; case 'b': gal_list_str_add(&p->bcols, strarr[i]+1, 0); break; default: error(EXIT_FAILURE, 0, "`%s' is not a valid value for `--outcols'. " "The first character of each value to this option must be " "either `a' or `b'. The former specifies a column from the " "first input and the latter a column from the second. The " "characters after them can be any column identifier (number, " "name, or regular expression). For more on column selection, " "please run this command:\n\n" " $ info gnuastro \"Selecting table columns\"\n", strarr[i]); } /* Revere the lists so they correspond to the input order. */ gal_list_str_reverse(&p->acols); gal_list_str_reverse(&p->bcols); } static void ui_preparations_out_name(struct matchparams *p) { if(p->logasoutput) { /* Set the logname (as output). */ if(p->cp.output) gal_checkset_allocate_copy(p->cp.output, &p->logname); else { if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) p->logname=gal_checkset_automatic_output(&p->cp, p->input1name, "_matched.txt"); else p->logname=gal_checkset_automatic_output(&p->cp, p->input1name, "_matched.fits"); } /* Make sure a file with this name doesn't exist. */ gal_checkset_writable_remove(p->out1name, 0, p->cp.dontdelete); } else { if(p->outcols) { if(p->cp.output==NULL) p->cp.output = gal_checkset_automatic_output(&p->cp, p->input1name, ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? "_matched.txt" : "_matched.fits") ); gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); } else { /* Set `p->out1name' and `p->out2name'. */ if(p->cp.output) { if( gal_fits_name_is_fits(p->cp.output) ) { gal_checkset_allocate_copy(p->cp.output, &p->out1name); gal_checkset_allocate_copy(p->cp.output, &p->out2name); } else { p->out1name=gal_checkset_automatic_output(&p->cp, p->cp.output, "_matched_1.txt"); p->out2name=gal_checkset_automatic_output(&p->cp, p->cp.output, "_matched_2.txt"); } } else { if(p->cp.tableformat==GAL_TABLE_FORMAT_TXT) { p->out1name=gal_checkset_automatic_output(&p->cp, p->input1name, "_matched_1.txt"); p->out2name=gal_checkset_automatic_output(&p->cp, p->input2name, "_matched_2.txt"); } else { p->out1name=gal_checkset_automatic_output(&p->cp, p->input1name, "_matched.fits"); gal_checkset_allocate_copy(p->out1name, &p->out2name); } } /* Make sure no file with these names exists. */ gal_checkset_writable_remove(p->out1name, 0, p->cp.dontdelete); gal_checkset_writable_remove(p->out2name, 0, p->cp.dontdelete); } /* If a log file is necessary, set its name here. */ if(p->cp.log) { p->logname = ( p->cp.tableformat==GAL_TABLE_FORMAT_TXT ? PROGRAM_EXEC".txt" : PROGRAM_EXEC".fits" ); gal_checkset_writable_remove(p->logname, 0, p->cp.dontdelete); } } } static void ui_preparations(struct matchparams *p) { /* Set the mode of the program. */ ui_set_mode(p); /* Currently Match only works on catalogs. */ if(p->mode==MATCH_MODE_WCS) error(EXIT_FAILURE, 0, "currently Match only works on catalogs, we will " "implement the WCS matching routines later"); else { ui_read_columns(p); if(p->outcols) ui_preparations_out_cols(p); } /* Set the output filename. */ ui_preparations_out_name(p); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct matchparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct matchparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->cp.hdu); free(p->out1name); free(p->out2name); free(p->cp.output); /* Print the final message. if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); */ } �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/main.c�����������������������������������������������������������������������0000644�0001750�0001750�00000003055�13211076737�013107� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Match - A program to match catalogs and WCS warps Match is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "match.h" /* Main function */ int main (int argc, char *argv[]) { struct timeval t1; struct matchparams p={{{0},0},0}; /* Set they starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ match(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/Makefile.in������������������������������������������������������������������0000644�0001750�0001750�00000211251�13217217705�014061� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; \ elif test -n '$(MAKE_HOST)'; then \ true; \ elif test -n '$(MAKE_VERSION)' && test -n '$(CURDIR)'; then \ true; \ else \ false; \ fi; \ } am__make_running_with_option = \ case $${target_option-} in \ ?) ;; \ *) echo "am__make_running_with_option: internal error: invalid" \ "target option '$${target_option-}' specified" >&2; \ exit 1;; \ esac; \ has_opt=no; \ 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@GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BIND = @GNULIB_BIND@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ 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uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/match/astmatch.conf����������������������������������������������������������������0000644�0001750�0001750�00000001731�13211076737�014471� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Match. # Match is part of GNU Astronomy Utilities. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astmatch --help # Full list of options, short doc. # $ astmatch -P # Print all options and used values. # $ info astmatch # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Input hdu2 1 # Catalog matching ccol1 2,3 ccol2 2,3���������������������������������������gnuastro-0.5/bin/match/Makefile.am������������������������������������������������������������������0000644�0001750�0001750�00000002560�13211076737�014053� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2017, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astmatch astmatch_LDADD = -lgnuastro astmatch_SOURCES = main.c ui.c match.c EXTRA_DIST = main.h authors-cite.h args.h ui.h match.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astmatch.conf ������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/������������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�011741� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/keywords.h��������������������������������������������������������������������0000644�0001750�0001750�00000002064�13121462410�013672� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef HEADER_H #define HEADER_H int keywords(struct fitsparams *p); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/fits.h������������������������������������������������������������������������0000644�0001750�0001750�00000002572�13121462410�012774� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef FITS_H #define FITS_H enum fits_action_ids { FITS_ACTION_INVALID, /* ==0: by C standard. */ FITS_ACTION_DELETE, FITS_ACTION_RENAME, FITS_ACTION_UPDATE, FITS_ACTION_WRITE, FITS_ACTION_COPY, FITS_ACTION_REMOVE, }; int fits_has_error(struct fitsparams *p, int actioncode, char *string, int status); int fits(struct fitsparams *p); #endif ��������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/ui.h��������������������������������������������������������������������������0000644�0001750�0001750�00000004021�13174462540�012447� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_EXTENSION = GAL_OPTIONS_GROUP_AFTER_COMMON, UI_GROUP_KEYWORD, }; /* Available letters for short options: b e f g i j l m n s v x y z A B E G J L O W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_REMOVE = 'R', UI_KEY_COPY = 'C', UI_KEY_CUT = 'k', UI_KEY_PRINTALLKEYS = 'p', UI_KEY_ASIS = 'a', UI_KEY_DELETE = 'd', UI_KEY_RENAME = 'r', UI_KEY_UPDATE = 'u', UI_KEY_WRITE = 'w', UI_KEY_COMMENT = 'c', UI_KEY_HISTORY = 'H', UI_KEY_DATE = 't', UI_KEY_QUITONERROR = 'Q', /* Only with long version (start with a value 1000, the rest will be set automatically). */ }; void ui_read_check_inputs_setup(int argc, char *argv[], struct fitsparams *p); void ui_free_and_report(struct fitsparams *p); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/args.h������������������������������������������������������������������������0000644�0001750�0001750�00000012517�13174462540�012777� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { { 0, 0, 0, 0, "HDUs (extensions):", UI_GROUP_EXTENSION }, { "remove", UI_KEY_REMOVE, "STR", 0, "Remove extension from input file.", UI_GROUP_EXTENSION, &p->remove, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "copy", UI_KEY_COPY, "STR", 0, "Copy extension to output file.", UI_GROUP_EXTENSION, &p->copy, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "cut", UI_KEY_CUT, "STR", 0, "Copy extension to output and remove from input.", UI_GROUP_EXTENSION, &p->cut, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Keywords (in one HDU):", UI_GROUP_KEYWORD }, { "asis", UI_KEY_ASIS, "STR", 0, "Write the argument string as is into the header.", UI_GROUP_KEYWORD, &p->asis, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "delete", UI_KEY_DELETE, "STR", 0, "Delete a keyword from the header.", UI_GROUP_KEYWORD, &p->delete, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "rename", UI_KEY_RENAME, "STR", 0, "Rename keyword, keeping value and comments.", UI_GROUP_KEYWORD, &p->rename, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "update", UI_KEY_UPDATE, "STR", 0, "Update a keyword value or comments.", UI_GROUP_KEYWORD, &p->update, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "write", UI_KEY_WRITE, "STR", 0, "Write a keyword (with value, comments and units).", UI_GROUP_KEYWORD, &p->write, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "history", UI_KEY_HISTORY, "STR", 0, "Add HISTORY keyword, any length is ok.", UI_GROUP_KEYWORD, &p->history, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "comment", UI_KEY_COMMENT, "STR", 0, "Add COMMENT keyword, any length is ok.", UI_GROUP_KEYWORD, &p->comment, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "date", UI_KEY_DATE, 0, 0, "Set the DATE keyword to the current time.", UI_GROUP_KEYWORD, &p->date, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "printallkeys", UI_KEY_PRINTALLKEYS, 0, 0, "Print all keywords in the selected HDU.", UI_GROUP_KEYWORD, &p->printallkeys, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "quitonerror", UI_KEY_QUITONERROR, 0, 0, "Quit if there is an error on any action.", GAL_OPTIONS_GROUP_OPERATING_MODE, &p->quitonerror, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/authors-cite.h����������������������������������������������������������������0000644�0001750�0001750�00000002774�13211076737�014457� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ����gnuastro-0.5/bin/fits/main.h������������������������������������������������������������������������0000644�0001750�0001750�00000005734�13161316532�012765� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include <gnuastro/list.h> #include <gnuastro/fits.h> #include <gnuastro-internal/options.h> /* Progarm name macros: */ #define PROGRAM_NAME "Fits" /* Program full name. */ #define PROGRAM_EXEC "astfits" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION enum fits_mode { FITS_MODE_INVALID, /* ==0, by C standard. */ FITS_MODE_HDU, FITS_MODE_KEY, }; /* Main program's structure */ struct fitsparams { /* From the environment. */ struct gal_options_common_params cp; /* Common parameters. */ int hdu_in_commandline; /* HDU wasn't given in config. file. */ char *filename; /* Name of input file. */ gal_list_str_t *remove; /* Remove extensions from a file. */ gal_list_str_t *copy; /* Copy extensions to output. */ gal_list_str_t *cut; /* Copy ext. to output and remove. */ uint8_t printallkeys; /* Print all the header keywords. */ uint8_t date; /* Set DATE to current time. */ char *comment; /* COMMENT value. */ char *history; /* HISTORY value. */ gal_list_str_t *asis; /* Strings to write asis. */ gal_list_str_t *delete; /* Keywords to remove. */ gal_list_str_t *rename; /* Rename a keyword. */ gal_list_str_t *update; /* For keywords to update. */ gal_list_str_t *write; /* Full arg. for keywords to add. */ uint8_t quitonerror; /* Quit if an error occurs. */ /* Internal: */ int mode; /* Operating on HDUs or keywords. */ gal_fits_list_key_t *write_keys; /* Keys to write in the header. */ gal_fits_list_key_t *update_keys; /* Keys to update in the header. */ time_t rawtime; /* Starting time of the program. */ }; #endif ������������������������������������gnuastro-0.5/bin/fits/keywords.c��������������������������������������������������������������������0000644�0001750�0001750�00000021243�13121462410�013665� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <stdlib.h> #include <gnuastro/fits.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "fits.h" /***********************************************************************/ /****************** Preparations ********************/ /***********************************************************************/ static void keywords_open(struct fitsparams *p, fitsfile **fptr, int iomode) { if(*fptr==NULL) *fptr=gal_fits_hdu_open(p->filename, p->cp.hdu, iomode); } /***********************************************************************/ /****************** File manipulation ********************/ /***********************************************************************/ static void keywords_rename_keys(struct fitsparams *p, fitsfile **fptr, int *r) { int status=0; char *copy, *str, *from, *to; /* Set the FITS file pointer. */ keywords_open(p, fptr, READWRITE); /* Tokenize the */ while(p->rename!=NULL) { /* Pop out the top element. */ str=gal_list_str_pop(&p->rename); /* Take a copy of the input string for error reporting, because `strtok' will write into the array. */ gal_checkset_allocate_copy(str, ©); /* Tokenize the input. */ from = strtok(str, ", "); to = strtok(NULL, ", "); /* Make sure both elements were read. */ if(from==NULL || to==NULL) error(EXIT_FAILURE, 0, "`%s' could not be tokenized in order to " "complete rename. There should be a space character " "or a comma (,) between the two keyword names. If you have " "used the space character, be sure to enclose the value to " "the `--rename' option in double quotation marks", copy); /* Rename the keyword */ fits_modify_name(*fptr, from, to, &status); if(status) *r=fits_has_error(p, FITS_ACTION_RENAME, from, status); /* Clean up the user's input string. Note that `strtok' just changes characters within the allocated string, no extra allocation is done. */ free(str); free(copy); } } static void keywords_write_update(struct fitsparams *p, fitsfile **fptr, gal_fits_list_key_t *keyll, int u1w2) { int status=0; gal_fits_list_key_t *tmp; /* Open the FITS file if it hasn't been opened yet. */ keywords_open(p, fptr, READWRITE); /* Go through each key and write it in the FITS file. */ while(keyll!=NULL) { /* Write the information: */ if(u1w2==1) { if(keyll->value) { if( fits_update_key(*fptr, gal_fits_type_to_datatype(keyll->type), keyll->keyname, keyll->value, keyll->comment, &status) ) gal_fits_io_error(status, NULL); } else { if(fits_write_key_null(*fptr, keyll->keyname, keyll->comment, &status)) gal_fits_io_error(status, NULL); } } else if (u1w2==2) { if(keyll->value) { if( fits_write_key(*fptr, gal_fits_type_to_datatype(keyll->type), keyll->keyname, keyll->value, keyll->comment, &status) ) gal_fits_io_error(status, NULL); } else { if(fits_write_key_null(*fptr, keyll->keyname, keyll->comment, &status)) gal_fits_io_error(status, NULL); } if(keyll->unit && fits_write_key_unit(*fptr, keyll->keyname, keyll->unit, &status) ) gal_fits_io_error(status, NULL); } else error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at `%s' so we " "can fix this problem. The value %d is not valid for `u1w2'", __func__, PACKAGE_BUGREPORT, u1w2); /* Add the unit (if one was given). */ if(keyll->unit && fits_write_key_unit(*fptr, keyll->keyname, keyll->unit, &status) ) gal_fits_io_error(status, NULL); /* Free the allocated spaces if necessary: */ if(keyll->vfree) free(keyll->value); if(keyll->kfree) free(keyll->keyname); if(keyll->cfree) free(keyll->comment); /* Keep the pointer to the next keyword and free the allocated space for this keyword.*/ tmp=keyll->next; free(keyll); keyll=tmp; } } static void keywords_print_all_keys(struct fitsparams *p, fitsfile **fptr) { size_t i=0; int nkeys, status=0; char *fullheader, *c, *cf; /* Open the FITS file. */ keywords_open(p, fptr, READONLY); /* Conver the header into a contiguous string. */ if( fits_hdr2str(*fptr, 0, NULL, 0, &fullheader, &nkeys, &status) ) gal_fits_io_error(status, NULL); /* FLEN_CARD supposes that the NULL string character is in the end of each keyword header card. In fits_hdr2str, the NULL characters are removed and so the maximum length is one less. */ cf=(c=fullheader)+nkeys*(FLEN_CARD-1); do { if(i && i%(FLEN_CARD-1)==0) putc('\n', stdout); putc(*c++, stdout); ++i; } while(c<cf); printf("\n"); if (fits_free_memory(fullheader, &status) ) gal_fits_io_error(status, "problem in header.c for freeing " "the memory used to keep all the headers"); } /***********************************************************************/ /****************** Main function ********************/ /***********************************************************************/ int keywords(struct fitsparams *p) { int status=0; int r=EXIT_SUCCESS; fitsfile *fptr=NULL; gal_list_str_t *tstll; /* Delete the requested keywords. */ if(p->delete) { keywords_open(p, &fptr, READWRITE); for(tstll=p->delete; tstll!=NULL; tstll=tstll->next) { fits_delete_key(fptr, tstll->v, &status); if(status) r=fits_has_error(p, FITS_ACTION_DELETE, tstll->v, status); } } /* Rename the requested keywords. */ if(p->rename) keywords_rename_keys(p, &fptr, &r); /* Update the requested keywords. */ if(p->update) keywords_write_update(p, &fptr, p->update_keys, 1); /* Write the requested keywords. */ if(p->write) keywords_write_update(p, &fptr, p->write_keys, 2); /* Put in any full line of keywords as-is. */ if(p->asis) for(tstll=p->asis; tstll!=NULL; tstll=tstll->next) { fits_write_record(fptr, tstll->v, &status); if(status) r=fits_has_error(p, FITS_ACTION_WRITE, tstll->v, status); } /* Add the history keyword(s). */ if(p->history) { fits_write_history(fptr, p->history, &status); if(status) r=fits_has_error(p, FITS_ACTION_WRITE, "HISTORY", status); } /* Add comment(s). */ if(p->comment) { fits_write_comment(fptr, p->comment, &status); if(status) r=fits_has_error(p, FITS_ACTION_WRITE, "COMMENT", status); } /* Update/add the date. */ if(p->date) { fits_write_date(fptr, &status); if(status) r=fits_has_error(p, FITS_ACTION_WRITE, "DATE", status); } /* If nothing was requested, then print all the keywords in this extension. */ if(p->printallkeys) keywords_print_all_keys(p, &fptr); /* Close the FITS file */ if(fits_close_file(fptr, &status)) gal_fits_io_error(status, NULL); /* Return. */ return r; } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/fits.c������������������������������������������������������������������������0000644�0001750�0001750�00000023640�13175442274�013005� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <errno.h> #include <error.h> #include <string.h> #include <gnuastro/list.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "fits.h" #include "keywords.h" int fits_has_error(struct fitsparams *p, int actioncode, char *string, int status) { char *action=NULL; int r=EXIT_SUCCESS; switch(actioncode) { case FITS_ACTION_DELETE: action="deleted"; break; case FITS_ACTION_RENAME: action="renamed"; break; case FITS_ACTION_UPDATE: action="updated"; break; case FITS_ACTION_WRITE: action="written"; break; case FITS_ACTION_COPY: action="copied"; break; case FITS_ACTION_REMOVE: action="renoved"; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at `%s' so we " "can fix this problem. The value of `actioncode' must not be %d", __func__, PACKAGE_BUGREPORT, actioncode); } if(p->quitonerror) { fits_report_error(stderr, status); error(EXIT_FAILURE, 0, "%s: not %s: %s\n", __func__, action, string); } else { fprintf(stderr, "Not %s: %s\n", action, string); r=EXIT_FAILURE; } return r; } /* Print all the extension informations. */ void fits_print_extension_info(struct fitsparams *p) { uint16_t *ui16; fitsfile *fptr; gal_data_t *cols=NULL, *tmp; char **tstra, **estra, **sstra; size_t i, numext, *dsize, ndim; int j, nc, numhdu, hdutype, status=0, type; char *msg, *tstr=NULL, sstr[1000], extname[FLEN_VALUE]; /* Open the FITS file and read the first extension type, upon moving to the next extension, we will read its type, so for the first we will need to do it explicitly. */ fptr=gal_fits_hdu_open(p->filename, "0", READONLY); if (fits_get_hdu_type(fptr, &hdutype, &status) ) gal_fits_io_error(status, "reading first extension"); /* Get the number of HDUs. */ if( fits_get_num_hdus(fptr, &numhdu, &status) ) gal_fits_io_error(status, "finding number of HDUs"); numext=numhdu; /* Allocate all the columns (in reverse order, since this is a simple linked list). */ gal_list_data_add_alloc(&cols, NULL, GAL_TYPE_STRING, 1, &numext, NULL, 1, p->cp.minmapsize, "HDU_SIZE", "name", "Size of " "image or table number of rows and columns."); gal_list_data_add_alloc(&cols, NULL, GAL_TYPE_STRING, 1, &numext, NULL, 1, p->cp.minmapsize, "HDU_TYPE", "name", "Image " "data type or `table' format (ASCII or binary)."); gal_list_data_add_alloc(&cols, NULL, GAL_TYPE_STRING, 1, &numext, NULL, 1, p->cp.minmapsize, "EXTNAME", "name", "Extension name of this HDU (EXTNAME in FITS)."); gal_list_data_add_alloc(&cols, NULL, GAL_TYPE_UINT16, 1, &numext, NULL, 1, p->cp.minmapsize, "HDU_INDEX", "count", "Index " "(starting from zero) of each HDU (extension)."); /* Keep pointers to the array of each column for easy writing. */ ui16 = cols->array; estra = cols->next->array; tstra = cols->next->next->array; sstra = cols->next->next->next->array; cols->next->disp_width=15; cols->next->next->disp_width=15; /* Fill in each column. */ for(i=0;i<numext;++i) { /* Work based on the type of the extension. */ switch(hdutype) { case IMAGE_HDU: gal_fits_img_info(fptr, &type, &ndim, &dsize, NULL, NULL); tstr=gal_type_name(type , 1); break; case ASCII_TBL: case BINARY_TBL: ndim=2; tstr = hdutype==ASCII_TBL ? "table_ascii" : "table_binary"; dsize=gal_data_malloc_array(GAL_TYPE_SIZE_T, 2, __func__, "dsize"); gal_fits_tab_size(fptr, dsize+1, dsize); break; default: error(EXIT_FAILURE, 0, "%s: a bug! the `hdutype' code %d not " "recognized", __func__, hdutype); } /* Read the extension name*/ fits_read_keyword(fptr, "EXTNAME", extname, NULL, &status); switch(status) { case 0: gal_fits_key_clean_str_value(extname); break; case KEY_NO_EXIST: sprintf(extname, "%s", GAL_BLANK_STRING); status=0; break; default: gal_fits_io_error(status, "reading EXTNAME keyword"); } status=0; /* Write the size into a string. `sprintf' returns the number of written characters (excluding the `\0'). So for each dimension's size that is written, we add to `nc' (the number of characters). Note that FITS allows blank extensions, in those cases, return "0". */ if(ndim>0) { nc=0; for(j=ndim-1;j>=0;--j) nc += sprintf(sstr+nc, "%zux", dsize[j]); sstr[nc-1]='\0'; free(dsize); } else { sstr[0]='0'; sstr[1]='\0'; } /* Write the strings into the columns. */ j=0; for(tmp=cols; tmp!=NULL; tmp=tmp->next) { switch(j) { case 0: ui16[i]=i; break; case 1: gal_checkset_allocate_copy(extname, estra+i); break; case 2: gal_checkset_allocate_copy(tstr, tstra+i); break; case 3: gal_checkset_allocate_copy(sstr, sstra+i); break; } ++j; } /* Move to the next extension if we aren't on the last extension. */ if( i!=numext-1 && fits_movrel_hdu(fptr, 1, &hdutype, &status) ) { asprintf(&msg, "moving to hdu %zu", i+1); gal_fits_io_error(status, msg); } } /* Print the resutls. */ if(!p->cp.quiet) { printf("%s\nRun on %s-----\n", PROGRAM_STRING, ctime(&p->rawtime)); printf("HDU (extension) information: `%s'.\n", p->filename); printf(" Column 1: Index (counting from 0, usable with `--hdu').\n"); printf(" Column 2: Name (`EXTNAME' in FITS standard, usable with " "`--hdu').\n"); printf(" Column 3: Image data type or `table' format (ASCII or " "binary).\n"); printf(" Column 4: Size of data in HDU.\n"); printf("-----\n"); } gal_table_write(cols, NULL, GAL_TABLE_FORMAT_TXT, NULL, NULL); gal_list_data_free(cols); } static void fits_hdu_remove(struct fitsparams *p, int *r) { char *hdu; fitsfile *fptr; int status=0, hdutype; while(p->remove) { /* Pop-out the top element. */ hdu=gal_list_str_pop(&p->remove); /* Open the FITS file at the specified HDU. */ fptr=gal_fits_hdu_open(p->filename, hdu, READWRITE); /* Delete the extension. */ if( fits_delete_hdu(fptr, &hdutype, &status) ) *r=fits_has_error(p, FITS_ACTION_REMOVE, hdu, status); /* Close the file. */ fits_close_file(fptr, &status); } } static void fits_hdu_copy(struct fitsparams *p, int cut1_copy0, int *r) { char *hdu; fitsfile *in, *out; int status=0, hdutype; gal_list_str_t *list = cut1_copy0 ? p->cut : p->copy; /* Open the output file. */ out=gal_fits_open_to_write(p->cp.output); /* Copy all the given extensions. */ while(list) { /* Pop-out the top element. */ hdu=gal_list_str_pop(&list); /* Open the FITS file at the specified HDU. */ in=gal_fits_hdu_open(p->filename, hdu, cut1_copy0 ? READWRITE : READONLY); /* Copy to the extension. */ if( fits_copy_hdu(in, out, 0, &status) ) *r=fits_has_error(p, FITS_ACTION_COPY, hdu, status); /* If this is a `cut' operation, then remove the extension. */ if(cut1_copy0) if( fits_delete_hdu(in, &hdutype, &status) ) *r=fits_has_error(p, FITS_ACTION_REMOVE, hdu, status); /* Close the input file. */ fits_close_file(in, &status); } /* Close the output file. */ fits_close_file(out, &status); } int fits(struct fitsparams *p) { int r=EXIT_SUCCESS, printhduinfo=1; switch(p->mode) { /* Keywords, we have a separate set of functions in `keywords.c'. */ case FITS_MODE_KEY: r=keywords(p); break; /* HDU, functions defined here. */ case FITS_MODE_HDU: if(p->copy) { fits_hdu_copy(p, 0, &r); printhduinfo=0; } if(p->cut) { fits_hdu_copy(p, 1, &r); printhduinfo=0; } if(p->remove) { fits_hdu_remove(p, &r); printhduinfo=0; } if(printhduinfo) fits_print_extension_info(p); break; /* Not recognized. */ default: error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to address " "the problem. The code %d is not recognized for p->mode", __func__, PACKAGE_BUGREPORT, p->mode); } return r; } ������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/extension.c�������������������������������������������������������������������0000644�0001750�0001750�00000001771�13121462410�014036� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> �������gnuastro-0.5/bin/fits/ui.c��������������������������������������������������������������������������0000644�0001750�0001750�00000034504�13211076737�012454� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/fits.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" allows you to view and " "manipulate (add, delete, or modify) FITS extensions (or HDUs) and FITS " "header keywords within one extension.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct fitsparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->keep = 1; cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* For clarity and non-zero initializations. */ p->mode = FITS_MODE_INVALID; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_TABLEFORMAT: case GAL_OPTIONS_KEY_DONTDELETE: case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_MINMAPSIZE: case GAL_OPTIONS_KEY_NUMTHREADS: cp->coptions[i].flags=OPTION_HIDDEN; break; case GAL_OPTIONS_KEY_OUTPUT: cp->coptions[i].doc="Output file name (only for writing HDUs)."; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct fitsparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: /* Only FITS files are acceptable. */ if( gal_fits_name_is_fits(arg) ) { if(p->filename) argp_error(state, "only one input file should be given"); else p->filename=arg; } else argp_error(state, "%s is not a recognized FITS file", arg); break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct fitsparams *p) { /* If any of the keyword manipulation options are requested, then set the mode flag to keyword-mode. */ if( p->date || p->comment || p->history || p->asis || p->delete || p->rename || p->update || p->write || p->printallkeys ) { /* Set the mode. */ p->mode=FITS_MODE_KEY; /* Check if a HDU is given. */ if(p->cp.hdu==NULL) error(EXIT_FAILURE, 0, "a HDU (extension) is necessary for keywrod " "related options but none was defined. Please use the " "`--hdu' (or `-h') option to select one"); } /* Same for the extension-related options */ if( p->remove || p->copy || p->cut ) { /* A small sanity check. */ if(p->mode!=FITS_MODE_INVALID) error(EXIT_FAILURE, 0, "extension and keyword manipulation options " "cannot be called together"); /* Set the mode and turn on the `needshdu' flag. */ p->mode=FITS_MODE_HDU; /* Make sure the output name is set. */ if(p->cp.output) gal_checkset_writable_remove(p->cp.output, 1, p->cp.dontdelete); else p->cp.output=gal_checkset_automatic_output(&p->cp, p->filename, "_ext.fits"); } /* If no options are given, go into HDU mode, which will print the HDU information when nothing is asked. */ if(p->mode==FITS_MODE_INVALID) { if(p->hdu_in_commandline) { p->printallkeys=1; p->mode = FITS_MODE_KEY; } else p->mode = FITS_MODE_HDU; } } static void ui_check_options_and_arguments(struct fitsparams *p) { /* Make sure an input file name was given and if it was a FITS file, that a HDU is also given. */ if(p->filename==NULL) error(EXIT_FAILURE, 0, "no input file is specified"); } /**************************************************************/ /***************** Preparations ********************/ /**************************************************************/ /* The `--update' and `--write' options take multiple values for each keyword, so here, we tokenize them and put them into a `gal_fits_list_key_t' list. */ static void ui_fill_fits_headerll(gal_list_str_t *input, gal_fits_list_key_t **output) { long l, *lp; void *fvalue; double d, *dp; gal_list_str_t *tmp; int i=0, type, vfree; char *c, *cf, *start, *tailptr; char *original, *keyname, *value, *comment, *unit; for(tmp=input; tmp!=NULL; tmp=tmp->next) { i=0; tailptr=NULL; /* `c' is created in case of an error, so the input value can be reported. */ errno=0; original=malloc(strlen(tmp->v)+1); if(original==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `original'", __func__, strlen(tmp->v)+1); strcpy(original, tmp->v); /* Tokenize the input. Note that strlen does not include the \0 character. So we have added it with a 1. */ cf=(c=start=tmp->v)+strlen(tmp->v)+1; keyname=value=comment=unit=NULL; do { switch(*c) { case ',': case '\0': *c='\0'; if(start!=c) switch(i) { case 0: keyname=start; break; case 1: value=start; break; case 2: comment=start; break; case 3: unit=start; break; default: error(EXIT_FAILURE, 0, "%s: only three commas should " "be given in the write or update keyword " "options. The general expected format is:\n" " KEYWORD,value,\"a comment string\",unit\n", original); } ++i; start=c+1; break; default: break; } } while(++c<cf); if(keyname==NULL) error(EXIT_FAILURE, 0, "the keyword in %s was not readable. " "The general expected format is:\n" " KEYWORD,value,\"a comment string\",unit\n" "Any space characters around the the comma (,) characters " "will be seen as part of the respective token", original); /* printf("\n\n-%s-\n-%s-\n-%s-\n-%s-\n", keyname, value, comment, unit); */ /* Find the of the value: */ errno=0; l=strtol(value, &tailptr, 10); if(*tailptr=='\0' && errno==0) { vfree=1; type=GAL_TYPE_INT64; errno=0; fvalue=lp=malloc(sizeof *lp); if(lp==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for `lp'", __func__, sizeof *lp); *lp=l; } else { errno=0; d=strtod(value, &tailptr); if(*tailptr=='\0' && errno==0) { vfree=1; type=GAL_TYPE_FLOAT64; errno=0; fvalue=dp=malloc(sizeof *dp); if(dp==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for " "`dp'", __func__, sizeof *dp); *dp=d; } else { fvalue=value; type=GAL_TYPE_STRING; vfree=0; } } gal_fits_key_list_add(output, type, keyname, 0, fvalue, vfree, comment, 0, unit); free(original); } } static void ui_preparations(struct fitsparams *p) { /* Fill in the key linked lists. We want to do this here so if there is any error in parsing the user's input, the error is reported before any change is made in the input file. */ if(p->write) ui_fill_fits_headerll(p->write, &p->write_keys); if(p->update) ui_fill_fits_headerll(p->update, &p->update_keys); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct fitsparams *p) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Check if the HDU is specified on the command-line. If so, then later, if no operation is requested, we will print the header of the given HDU.*/ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) if(cp->coptions[i].key==GAL_OPTIONS_KEY_HDU && cp->coptions[i].set) p->hdu_in_commandline=1; /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_and_report(struct fitsparams *p) { /* Free the allocated arrays: */ free(p->cp.output); } ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/main.c������������������������������������������������������������������������0000644�0001750�0001750�00000002753�13121462410�012747� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Fits - View and manipulate FITS extensions and/or headers. Fits is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "fits.h" int main (int argc, char *argv[]) { int r; struct fitsparams p={{{0},0},0}; /* Get the starting time. */ time(&p.rawtime); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ r=fits(&p); /* Free all non-freed allocations. */ ui_free_and_report(&p); /* Return successfully.*/ return r; } ���������������������gnuastro-0.5/bin/fits/Makefile.in�������������������������������������������������������������������0000644�0001750�0001750�00000211572�13217217705�013740� 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@GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BIND = @GNULIB_BIND@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINDOWS_STAT_INODES = @WINDOWS_STAT_INODES@ WINDOWS_STAT_TIMESPEC = @WINDOWS_STAT_TIMESPEC@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Fits. # Fits is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astfits --help # Full list of options, short doc. # $ astfits -P # Print all options and used values. # $ info astfits # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. �����������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/fits/Makefile.am�������������������������������������������������������������������0000644�0001750�0001750�00000002630�13121462410�013705� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astfits astfits_LDADD = -lgnuastro astfits_SOURCES = main.c ui.c extension.c fits.c keywords.c EXTRA_DIST = main.h authors-cite.h args.h ui.h extension.c fits.h keywords.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astfits.conf ��������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/������������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�011737� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/onecrop.h���������������������������������������������������������������������0000644�0001750�0001750�00000005245�13216276304�013504� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ONECROP_H #define ONECROP_H #include <fitsio.h> #include <gnuastro/threads.h> struct onecropparams { void *array; /* Pointer to basic structure: */ struct cropparams *p; /* About input image. */ size_t in_ind; /* Index of this image in the input names. */ fitsfile *infits; /* Pointer to the input FITS image. */ long fpixel[2]; /* Position of first pixel in input image. */ long lpixel[2]; /* Position of last pixel in input image. */ double *ipolygon; /* Input image based polygon vertices. */ /* Output (cropped) image. */ size_t out_ind; /* Index of this crop in the output list. */ double world[2]; /* World coordinates of crop center. */ double sized[2]; /* Width and height of image in degrees. */ double corners[8]; /* RA and Dec of this crop's four sides. */ double equatorcorr[2]; /* Crop crosses the equator, see wcsmode.c. */ fitsfile *outfits; /* Pointer to the output FITS image. */ /* For log */ char *name; /* Filename of crop. */ size_t numimg; /* Number of images used to make this crop. */ unsigned char centerfilled; /* ==1 if the center is filled. */ /* Thread parameters. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* pthread barrier to keep threads waiting. */ }; void onecrop_parse_polygon(struct cropparams *p); void onecrop_name(struct onecropparams *crp); void onecrop(struct onecropparams *crp); int onecrop_center_filled(struct onecropparams *crp); void crop_print_log(struct onecropparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/wcsmode.h���������������������������������������������������������������������0000644�0001750�0001750�00000002360�13124524246�013472� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef WCSMODE_H #define WCSMODE_H void wcsmode_check_prepare(struct cropparams *p, struct inputimgs *img); void wcsmode_crop_corners(struct onecropparams *crp); void fillcrpipolygon(struct onecropparams *crp); int wcsmode_overlap(struct onecropparams *crp); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/crop.h������������������������������������������������������������������������0000644�0001750�0001750�00000002056�13121462410�012765� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef IMGMODE_H #define IMGMODE_H void crop(struct cropparams *p); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/ui.h��������������������������������������������������������������������������0000644�0001750�0001750�00000004214�13174462540�012451� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_CENTER_GENERAL = GAL_OPTIONS_GROUP_AFTER_COMMON, UI_GROUP_CENTER_SINGLE, UI_GROUP_CENTER_CATALOG, UI_GROUP_REGION, }; /* Available letters for short options: a d e f g i j k m r t u v y A B E G H J L Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_CATALOG = 'C', UI_KEY_NOBLANK = 'b', UI_KEY_SUFFIX = 'p', UI_KEY_NAMECOL = 'n', UI_KEY_SECTION = 's', UI_KEY_POLYGON = 'l', UI_KEY_ZEROISNOTBLANK = 'z', UI_KEY_MODE = 'O', UI_KEY_WIDTH = 'w', UI_KEY_CENTER = 'c', UI_KEY_COORDCOL = 'x', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_CATHDU = 1000, UI_KEY_HSTARTWCS, UI_KEY_HENDWCS, UI_KEY_OUTPOLYGON, UI_KEY_CHECKCENTER, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct cropparams *p); void ui_free_report(struct cropparams *p, struct timeval *t1); #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/args.h������������������������������������������������������������������������0000644�0001750�0001750�00000015123�13211076737�012772� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { /* Input. */ { "mode", UI_KEY_MODE, "STR", 0, "Coordinate mode `img' or `wcs'.", GAL_OPTIONS_GROUP_INPUT, &p->mode, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET, ui_parse_coordinate_mode }, { "hstartwcs", UI_KEY_HSTARTWCS, "INT", 0, "Header keyword number to start reading WCS.", GAL_OPTIONS_GROUP_INPUT, &p->hstartwcs, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "hendwcs", UI_KEY_HENDWCS, "INT", 0, "Header keyword number to stop reading WCS.", GAL_OPTIONS_GROUP_INPUT, &p->hendwcs, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "zeroisnotblank", UI_KEY_ZEROISNOTBLANK, 0, 0, "0.0 in float or double images are not blank.", GAL_OPTIONS_GROUP_INPUT, &p->zeroisnotblank, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Output. */ { "noblank", UI_KEY_NOBLANK, 0, 0, "Remove parts of the crop box out of input image.", GAL_OPTIONS_GROUP_OUTPUT, &p->noblank, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "suffix", UI_KEY_SUFFIX, "STR", 0, "Suffix (postfix) of cropped images.", GAL_OPTIONS_GROUP_OUTPUT, &p->suffix, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Crop by center", UI_GROUP_CENTER_GENERAL }, { "checkcenter", UI_KEY_CHECKCENTER, "INT", 0, "Width (in pixels) of box at center to check.", UI_GROUP_CENTER_GENERAL, &p->checkcenter, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_0_OR_ODD, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "width", UI_KEY_WIDTH, "FLT[,...]", 0, "Width when crop is defined by its center.", UI_GROUP_CENTER_GENERAL, &p->width, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, { "center", UI_KEY_CENTER, "FLT[,...]", 0, "Central coordinates of a single crop.", UI_GROUP_CENTER_GENERAL, &p->center, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, gal_options_parse_csv_float64 }, { 0, 0, 0, 0, "Crop by center (when a catalog is given)", UI_GROUP_CENTER_CATALOG }, { "catalog", UI_KEY_CATALOG, "STR", 0, "Input catalog filename.", UI_GROUP_CENTER_CATALOG, &p->catname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "cathdu", UI_KEY_CATHDU, "STR/INT", 0, "HDU of catalog, if it is a FITS table.", UI_GROUP_CENTER_CATALOG, &p->cathdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "namecol", UI_KEY_NAMECOL, "STR/INT", 0, "Column no./info of crop filename (no suffix).", UI_GROUP_CENTER_CATALOG, &p->namecol, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "coordcol", UI_KEY_COORDCOL, "STR/INT", 0, "Column no./info containing coordinates.", UI_GROUP_CENTER_CATALOG, &p->coordcol, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Crop by region", UI_GROUP_REGION }, { "section", UI_KEY_SECTION, "STR", 0, "Image section string specifying crop range.", UI_GROUP_REGION, &p->section, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "polygon", UI_KEY_POLYGON, "STR", 0, "Polygon vertices of region to crop, keep inside.", UI_GROUP_REGION, &p->polygon, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "outpolygon", UI_KEY_OUTPOLYGON, 0, 0, "Keep the polygon's outside, mask the inside.", UI_GROUP_REGION, &p->outpolygon, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Operating mode */ {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/authors-cite.h����������������������������������������������������������������0000644�0001750�0001750�00000002767�13211076737�014457� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ���������gnuastro-0.5/bin/crop/main.h������������������������������������������������������������������������0000644�0001750�0001750�00000012314�13216276304�012756� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "Crop" /* Program full name. */ #define PROGRAM_EXEC "astcrop" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Macros */ #define LOGFILENAME PROGRAM_EXEC".log" #define FILENAME_BUFFER_IN_VERB 30 #define MAXDIM 2 /* Modes to interpret coordinates. */ enum crop_modes { IMGCROP_MODE_INVALID, /* For sanity checks. */ IMGCROP_MODE_IMG, /* Use image coordinates. */ IMGCROP_MODE_WCS, /* Use WCS coordinates. */ }; /* The sides of the image keep the celestial coordinates of the four sides of this image. With respect to the pixels they are. */ struct inputimgs { char *name; /* File name of input image. */ size_t ndim; /* Number of dimensions of this image. */ size_t *dsize; /* Size of the image. */ int nwcs; /* Number of WCS in each input image. */ struct wcsprm *wcs; /* WCS structure of each input image. */ char *wcstxt; /* Text output of each WCS. */ int nwcskeys; /* Number of keywords in the header WCS. */ double corners[8]; /* RA and Dec of this image corners (within). */ double sized[2]; /* Width and height of image in degrees. */ double equatorcorr[2]; /* If image crosses the equator, see wcsmode.c.*/ }; /* Main program parameters: */ struct cropparams { /* Directly from command-line */ struct gal_options_common_params cp; /* Common parameters. */ gal_list_str_t *inputs; /* All input FITS files. */ size_t hstartwcs; /* Header keyword No. to start read WCS. */ size_t hendwcs; /* Header keyword No. to end read WCS. */ int mode; /* Image or WCS mode. */ uint8_t zeroisnotblank; /* ==1: In float or double, keep 0.0. */ uint8_t noblank; /* ==1: no blank (out of image) pixels. */ char *suffix; /* Ending of output file name. */ size_t checkcenter; /* width of a box to check for zeros */ gal_data_t *center; /* Center position of crop. */ gal_data_t *width; /* Width of crop when defined by center. */ char *catname; /* Name of input catalog. */ char *cathdu; /* HDU of catalog if its a FITS file. */ char *namecol; /* Filename (without suffix) of crop col.*/ gal_list_str_t *coordcol; /* Column in catalog with coordinates. */ char *section; /* Section string. */ char *polygon; /* Input string of polygon vertices. */ uint8_t outpolygon; /* ==1: Keep the inner polygon region. */ /* Internal */ size_t numin; /* Number of input images. */ size_t numout; /* Number of output images. */ double **centercoords; /* The center coordinates. */ char **name; /* filename of crop in row. */ double *wpolygon; /* Array of WCS polygon vertices. */ double *ipolygon; /* Array of image polygon vertices. */ size_t nvertices; /* Number of polygon vertices. */ long iwidth[2]; /* Image mode width (in pixels). */ double *pixscale; /* Resolution in each dimension. */ time_t rawtime; /* Starting time of the program. */ int outnameisfile; /* Output filename is a directory. */ int type; /* Type of output(s). */ void *bitnul; /* Null value for this data-type. */ struct inputimgs *imgs; /* WCS and size information for inputs. */ gal_data_t *log; /* Log file contents. */ }; #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/onecrop.c���������������������������������������������������������������������0000644�0001750�0001750�00000065337�13216276304�013507� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <ctype.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <float.h> #include <string.h> #include <stdlib.h> #include <gnuastro/box.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/polygon.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "onecrop.h" #include "wcsmode.h" /*******************************************************************/ /************ Set/correct first and last pixel **************/ /*******************************************************************/ /* Read the section string and set the starting and ending pixels based on that. */ void onecrop_parse_section(struct cropparams *p, size_t *dsize, long *fpixel, long *lpixel) { int add; long read; char *tailptr; char forl='f', *pt=p->section; long naxes[2]={dsize[1], dsize[0]}; size_t i, dim=0, ndim=p->imgs->ndim; /* When the user asks for a section of the dataset, then the cropped region is not defined by its center. So it makes no sense to later check if the center is blank or not. Hence, we will over-write it with zero. */ p->checkcenter=0; /* Initialize the fpixel and lpixel arrays (note that `section' is only defined in image mode, so there will only be one element in `imgs'. */ for(i=0;i<ndim;++i) { fpixel[i] = 1; lpixel[i] = naxes[i] = p->imgs->dsize[ ndim - i - 1 ]; } /* Parse the string. */ while(*pt!='\0') { add=0; switch(*pt) { case ',': ++dim; if(dim>=ndim) error(EXIT_FAILURE, 0, "Extra `,` in `%s`", p->section); forl='f'; ++pt; break; case ':': forl='l'; ++pt; break; case '.': error(EXIT_FAILURE, 0, "the numbers in the argument to " "`--section` (`-s') have to be integers. You input " "includes a float number: %s", p->section); break; case ' ': case '\t': ++pt; break; case '*': add=1; /* If it is an asterisk, then add the */ ++pt; /* given value to the maximum size of */ break; /* the image. */ default: break; } /* Read the number: */ read=strtol(pt, &tailptr, 0); /* Check if there actually was a number. printf("\n\n------\n%c: %ld (%s)\n", *pt, read, tailptr); */ /* Make sure if a number was read at all? */ if(tailptr==pt) /* No number was read! */ { if(add) read=0; /* We have a * followed by `:' or `,'. */ else continue; } /* Put it in the correct array. */ if(forl=='f') fpixel[dim] = add ? naxes[dim]+read : read; else lpixel[dim] = add ? naxes[dim]+read : read; pt=tailptr; } /* Make sure the first pixel is located before/below the last pixel. */ for(i=0;i<ndim;++i) if(fpixel[i]>lpixel[i]) error(EXIT_FAILURE, 0, "the bottom left corner coordinates " "cannot be larger or equal to the top right's! Your section " "string (%s) has been read as: bottom left coordinate " "(%ld, %ld) to top right coordinate (%ld, %ld)", p->section, fpixel[0], fpixel[1], lpixel[0], lpixel[1]); /* For a check: printf("\n%s\n", p->section); printf("fpixel: ("); for(i=0;i<ndim;++i) printf("%ld, ", fpixel[i]); printf("\b\b)\n"); printf("lpixel: ("); for(i=0;i<ndim;++i) printf("%ld, ", lpixel[i]); printf("\b\b)\n\n"); exit(0); */ } void onecrop_parse_polygon(struct cropparams *p) { size_t dim=0; char *tailptr; char *pt=p->polygon; double read, *array; gal_list_f64_t *vertices=NULL; /* If control reached here, then the cropped region is not defined by its center. So it makes no sense to check if the center is blank. */ p->checkcenter=0; /* Parse the string. */ while(*pt!='\0') { switch(*pt) { case ',': ++dim; if(dim==2) error(EXIT_FAILURE, 0, "Extra `,` in `%s`", p->polygon); ++pt; break; case ':': if(dim==0) error(EXIT_FAILURE, 0, "not enough coordinates for at least " "one polygon vertex (in %s)", p->polygon); dim=0; ++pt; break; default: break; } /* strtod will skip white spaces if they are before a number, but not when they are before a : or ,. So we need to remove all white spaces. White spaces are usually put beside each other, so if one is encountered, go along the string until the white space characters finish. */ if(isspace(*pt)) ++pt; else { /* Read the number: */ read=strtod(pt, &tailptr); /* Check if there actually was a number. printf("\n\n------\n%zu: %f (%s)\n", dim, read, tailptr); */ /* Make sure if a number was read at all? */ if(tailptr==pt) /* No number was read! */ error(EXIT_FAILURE, 0, "%s could not be parsed as a floating " "point number", tailptr); /* Check if there are no extra characters in the number, for example we don't have a case like `1.00132.17', or 1.01i:2.0. Such errors are not uncommon when typing large numbers, and if ignored, they can lead to unpredictable results, so its best to abort and inform the user. */ if( *tailptr!='\0' && !isspace(*tailptr) && strchr(":,", *tailptr)==NULL ) error(EXIT_FAILURE, 0, "'%s' is an invalid floating point number " "sequence in the value to the `--polygon' option, error " "detected at '%s'", pt, tailptr); /* Add the read coordinate to the list of coordinates. */ gal_list_f64_add(&vertices, read); /* The job here is done, start from tailptr */ pt=tailptr; } } /* Put the coordinates into an array while reversing their order so they correspond to the user's order, then put it in the right place.*/ array=gal_list_f64_to_array(vertices, 1, &p->nvertices); if(p->mode==IMGCROP_MODE_IMG) { p->ipolygon=array; p->wpolygon=NULL; } else { p->ipolygon=NULL; p->wpolygon=array; } /* The number of vertices is actually the number of nodes in the list divided by the dimension of the dataset (note that we were counting the dimension from 0. */ p->nvertices/=(dim+1); /* For a check: { size_t i; double *polygon=p->mode==IMGCROP_MODE_IMG?p->ipolygon:p->wpolygon; for(i=0;i<p->nvertices;++i) printf("(%f, %f)\n", polygon[i*2], polygon[i*2+1]); } exit(0); */ /* Clean up: */ gal_list_f64_free(vertices); } void onecrop_ipolygon_fl(double *ipolygon, size_t nvertices, long *fpixel, long *lpixel) { size_t i; double minx=FLT_MAX, miny=FLT_MAX; double maxx=-FLT_MAX, maxy=-FLT_MAX; /* Find their minimum and maximum values. */ for(i=0;i<nvertices;++i) { if(ipolygon[i*2]>maxx) maxx=ipolygon[i*2]; if(ipolygon[i*2]<minx) minx=ipolygon[i*2]; if(ipolygon[i*2+1]>maxy) maxy=ipolygon[i*2+1]; if(ipolygon[i*2+1]<miny) miny=ipolygon[i*2+1]; } /* Set the first and last pixel. */ fpixel[0] = minx - (int)minx >=0.5 ? (int)minx + 1 : (int)minx; fpixel[1] = miny - (int)miny >=0.5 ? (int)miny + 1 : (int)miny; lpixel[0] = maxx - (int)maxx >=0.5 ? (int)maxx + 1 : (int)maxx; lpixel[1] = maxy - (int)maxy >=0.5 ? (int)maxy + 1 : (int)maxy; } #define POLYGON_MASK(CTYPE) { \ CTYPE *ba=array, *bb=gal_blank_alloc_write(type); \ for(i=0;i<size;++i) \ { \ point[0]=i%s1+1; point[1]=i/s1+1; \ if(gal_polygon_pin(ipolygon, point, nvertices)==outpolygon) \ ba[i]=*bb; \ } \ free(bb); \ } void polygonmask(struct onecropparams *crp, void *array, long *fpixel_i, size_t s0, size_t s1) { int type=crp->p->type; double *ipolygon, point[2]; int outpolygon=crp->p->outpolygon; size_t i, *ordinds, size=s0*s1, nvertices=crp->p->nvertices; /* First of all, allocate enough space to put a copy of the input coordinates (we will be using that after sorting in an anti-clickwise manner.) */ errno=0; ipolygon=malloc(2*nvertices*sizeof *ipolygon); if(ipolygon==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for ipolygon", __func__, 2*nvertices*sizeof *ipolygon); errno=0; ordinds=malloc(nvertices*sizeof *ordinds); if(ordinds==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for ordinds", __func__, nvertices*sizeof *ordinds); /* Find the order of the polygons and put the elements in the proper order. Also subtract the fpixel_i coordinates from all the vertices to bring them into the crop image coordinates.*/ gal_polygon_ordered_corners(crp->ipolygon, crp->p->nvertices, ordinds); for(i=0;i<crp->p->nvertices;++i) { ipolygon[i*2 ] = crp->ipolygon[ordinds[i]*2] - fpixel_i[0]; ipolygon[i*2+1] = crp->ipolygon[ordinds[i]*2+1] - fpixel_i[1]; } /* Go over all the pixels in the image and if they are within the polygon keep them if the user has asked for it.*/ switch(type) { case GAL_TYPE_UINT8: POLYGON_MASK(uint8_t); break; case GAL_TYPE_INT8: POLYGON_MASK(int8_t); break; case GAL_TYPE_UINT16: POLYGON_MASK(uint16_t); break; case GAL_TYPE_INT16: POLYGON_MASK(int16_t); break; case GAL_TYPE_UINT32: POLYGON_MASK(uint32_t); break; case GAL_TYPE_INT32: POLYGON_MASK(int32_t); break; case GAL_TYPE_INT64: POLYGON_MASK(int64_t); break; case GAL_TYPE_FLOAT32: POLYGON_MASK(float); break; case GAL_TYPE_FLOAT64: POLYGON_MASK(double); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s, so we " "can fix the problem. Type code %d is not recognized", __func__, PACKAGE_BUGREPORT, type); } /* Clean up: */ free(ordinds); free(ipolygon); } /*******************************************************************/ /****************** One crop. *********************/ /*******************************************************************/ static void onecrop_zero_to_nan(void *array, size_t size, int type) { float *fp, *ffp; double *dp, *fdp; switch(type) { case GAL_TYPE_FLOAT32: ffp=(fp=array)+size; do if(*fp==0.0f) *fp=NAN; while(++fp<ffp); break; case GAL_TYPE_FLOAT64: fdp=(dp=array)+size; do if(*dp==0.0f) *dp=NAN; while(++dp<fdp); break; default: error(EXIT_FAILURE, 0, "%s: %d is not a recognized type", __func__, type); } } /* Set the output name and image output sizes. */ void onecrop_name(struct onecropparams *crp) { char **strarr; struct cropparams *p=crp->p; struct gal_options_common_params *cp=&p->cp; /* Set the output name and crop sides: */ if(p->catname) { /* If a name column was set, use it, otherwise, use the ID of the profile. */ if(p->name) { strarr=p->name; asprintf(&crp->name, "%s%s%s", cp->output, strarr[crp->out_ind], p->suffix); } else asprintf(&crp->name, "%s%zu%s", cp->output, crp->out_ind+1, p->suffix); /* Make sure the file doesn't exist. */ gal_checkset_writable_remove(crp->name, 0, cp->dontdelete); } else { /* Set the output name. */ if(p->outnameisfile) /* An output file was specified. */ { crp->name=cp->output; gal_checkset_writable_remove(crp->name, 0, cp->dontdelete); } else /* The output was a directory, use automatic output. */ crp->name=gal_checkset_automatic_output(cp, p->imgs[crp->in_ind].name, p->suffix); } } /* Find the first and last pixel of a crop. */ static void onecrop_flpixel(struct onecropparams *crp) { struct cropparams *p=crp->p; size_t ndim=p->imgs->ndim; double center[MAXDIM]; int ncoord=1, status=0; size_t i, *dsize=p->imgs[crp->in_ind].dsize; long *fpixel=crp->fpixel, *lpixel=crp->lpixel; double pixcrd[MAXDIM], imgcrd[MAXDIM], phi[1], theta[1]; switch(p->mode) { case IMGCROP_MODE_IMG: if(p->section) /* Defined by section. */ onecrop_parse_section(p, dsize, fpixel, lpixel); else if(p->polygon) /* Defined by polygon. */ { if(p->outpolygon==0) onecrop_ipolygon_fl(p->ipolygon, p->nvertices, fpixel, lpixel); } else { for(i=0;i<ndim;++i) center[i] = p->centercoords[i][crp->out_ind]; gal_box_border_from_center(center, ndim, p->iwidth, fpixel, lpixel); } break; case IMGCROP_MODE_WCS: /* In wcsmode, crp->world is already filled. */ if(p->polygon) /* Note: p->iwidth was set based on p->wwidth. */ { /* Fill crp->ipolygon in wcspolygonpixel, then set flpixel*/ fillcrpipolygon(crp); if(p->outpolygon==0) onecrop_ipolygon_fl(crp->ipolygon, p->nvertices, fpixel, lpixel); } else { /* Convert `crp->world' (in WCS) into `pixcrd' (image coord). */ if(wcss2p(p->imgs[crp->in_ind].wcs, ncoord, ndim, crp->world, phi, theta, imgcrd, pixcrd, &status) ) if(status) error(EXIT_FAILURE, 0, "%s: wcss2p error %d: %s", __func__, status, wcs_errmsg[status]); /* Find the first and last pixels of this crop. */ gal_box_border_from_center(pixcrd, ndim, p->iwidth, fpixel, lpixel); } break; default: error(EXIT_FAILURE, 0, "%s: a bug! The domain (WCS or image) are not " "set. Please contact us at %s so we can see how it got to this " "impossible place", __func__, PACKAGE_BUGREPORT); } /* If the user only wants regions outside to the polygon, then set the fpixel and lpixel to cover the full input image. */ if(p->polygon && p->outpolygon) { crp->fpixel[0]=crp->fpixel[1]=1; crp->lpixel[0]=dsize[1]; crp->lpixel[1]=dsize[0]; } } /* Find the size of the final FITS image (irrespective of how many crops will be needed for it) and make the image to keep the data. NOTE: The fpixel and lpixel in crp keep the first and last pixel of the total image for this crop, irrespective of the final keeping blank areas or not. While the fpixel_i and lpixel_i arrays keep the first and last pixels after the blank pixels have been removed. */ static void onecrop_make_array(struct onecropparams *crp, long *fpixel_i, long *lpixel_i, long *fpixel_c, long *lpixel_c) { double crpix; fitsfile *ofp; long naxes[MAXDIM]; char *outname=crp->name; int status=0, type=crp->p->type; size_t i, ndim=crp->p->imgs->ndim; char **strarr, cpname[FLEN_KEYWORD]; gal_data_t *rkey=gal_data_array_calloc(1); char *cp, *cpf, blankrec[80], titlerec[80]; struct inputimgs *img=&crp->p->imgs[crp->in_ind]; /* Set the last element of the blank array. */ cpf=blankrec+79; *cpf='\0'; titlerec[79]='\0'; cp=blankrec; do *cp=' '; while(++cp<cpf); /* Set the size of the output, in WCS mode, noblank==0. */ if(crp->p->noblank && crp->p->mode==IMGCROP_MODE_IMG) for(i=0;i<ndim;++i) { fpixel_c[i] = 1; lpixel_c[i] = naxes[i] = lpixel_i[i]-fpixel_i[i]+1; } else for(i=0;i<ndim;++i) naxes[i] = crp->lpixel[i]-crp->fpixel[i]+1; /* Create the FITS file with a blank first extension, then close it, so with the next `fits_open_file', we build the image in the second extension. This way, atleast for Gnuastro's outputs, we can consistently use `-h1' (something like how you count columns, or generally everything from 1). */ if(fits_create_file(&ofp, outname, &status)) gal_fits_io_error(status, "creating file"); fits_create_img(ofp, SHORT_IMG, 0, naxes, &status); fits_close_file(ofp, &status); /* Create the output crop image. */ fits_open_file(&crp->outfits, outname, READWRITE, &status); fits_create_img(crp->outfits, gal_fits_type_to_bitpix(type), ndim, naxes, &status); gal_fits_io_error(status, "creating image"); ofp=crp->outfits; /* When CFITSIO creates a FITS extension it adds two comments linking to the FITS paper. Since we are mentioning the version of CFITSIO and only use its ruitines to read/write from/to FITS files, this is redundant. If `status!=0', then `gal_fits_io_error' will abort, but in case CFITSIO doesn't write the comments, status will become non-zero. So we are resetting it to zero after these (because not being able to delete them isn't an error). */ fits_delete_key(ofp, "COMMENT", &status); fits_delete_key(ofp, "COMMENT", &status); status=0; /* Read the units of the input dataset and store them in the output. */ rkey->next=NULL; rkey->name="BUNIT"; rkey->type=GAL_TYPE_STRING; gal_fits_key_read_from_ptr(crp->infits, rkey, 1, 1); if(rkey->status==0) /* The BUNIT keyword was read. */ { strarr=rkey->array; fits_update_key(ofp, TSTRING, "BUNIT", strarr[0], "physical units", &status); gal_fits_io_error(status, "writing BUNIT"); } rkey->name=NULL; /* `name' wasn't allocated. */ gal_data_free(rkey); /* Write the blank value as a FITS keyword if necessary. */ if( type!=GAL_TYPE_FLOAT32 && type!=GAL_TYPE_FLOAT64 ) if(fits_write_key(ofp, gal_fits_type_to_datatype(crp->p->type), "BLANK", crp->p->bitnul, "pixels with no data", &status) ) gal_fits_io_error(status, "adding Blank"); if(fits_write_null_img(ofp, 1, naxes[0]*naxes[1], &status)) gal_fits_io_error(status, "writing null array"); /* Write the WCS header keywords in the output FITS image, then update the header keywords. */ if(img->wcs) { /* Write the WCS title and common WCS information. */ if(fits_write_record(ofp, blankrec, &status)) gal_fits_io_error(status, NULL); sprintf(titlerec, "%sWCS information", GAL_FITS_KEY_TITLE_START); for(i=strlen(titlerec);i<79;++i) titlerec[i]=' '; fits_write_record(ofp, titlerec, &status); for(i=0;i<img->nwcskeys-1;++i) fits_write_record(ofp, &img->wcstxt[i*80], &status); gal_fits_io_error(status, NULL); /* Correct the CRPIX keywords. */ for(i=0;i<ndim;++i) { sprintf(cpname, "CRPIX%zu", i+1); crpix = img->wcs->crpix[i] - (fpixel_i[i]-1) + (fpixel_c[i]-1); fits_update_key(ofp, TDOUBLE, cpname, &crpix, NULL, &status); gal_fits_io_error(status, NULL); } } /* Add the Crop information. */ sprintf(titlerec, "%sCrop information", GAL_FITS_KEY_TITLE_START); for(i=strlen(titlerec);i<79;++i) titlerec[i]=' '; if(fits_write_record(ofp, titlerec, &status)) gal_fits_io_error(status, NULL); } /* The starting and ending points are set in the onecropparams structure for one crop from one image. Crop that region out of the input. */ void onecrop(struct onecropparams *crp) { struct cropparams *p=crp->p; struct inputimgs *img=&p->imgs[crp->in_ind]; void *array; int status=0, anynul=0; char basename[FLEN_KEYWORD]; fitsfile *ifp=crp->infits, *ofp; gal_fits_list_key_t *headers=NULL; size_t i, j, cropsize=1, ndim=img->ndim; char region[FLEN_VALUE], regionkey[FLEN_KEYWORD]; long fpixel_o[MAXDIM], lpixel_o[MAXDIM], inc[MAXDIM]; long naxes[MAXDIM], fpixel_i[MAXDIM] , lpixel_i[MAXDIM]; /* Fill the `naxes' and `inc' arrays. */ for(i=0;i<ndim;++i) { inc[ i ] = 1; naxes[ i ] = img->dsize[ ndim - i - 1 ]; } /* Find the first and last pixel of this crop box from this input image. Then copy the first and last pixels into the `_i' arrays.*/ onecrop_flpixel(crp); memcpy(fpixel_i, crp->fpixel, ndim*sizeof *fpixel_i); memcpy(lpixel_i, crp->lpixel, ndim*sizeof *lpixel_i); /* Find the overlap and apply it if there is any overlap. */ if( gal_box_overlap(naxes, fpixel_i, lpixel_i, fpixel_o, lpixel_o, ndim) ) { /* Make the output FITS image and initialize it with an array of NaN or BLANK values. */ if(crp->outfits==NULL) onecrop_make_array(crp, fpixel_i, lpixel_i, fpixel_o, lpixel_o); ofp=crp->outfits; /* Allocate an array to keep the desired crop region, then read the desired pixels onto it. */ status=0; for(i=0;i<ndim;++i) cropsize *= ( lpixel_i[i] - fpixel_i[i] + 1 ); array=gal_data_malloc_array(p->type, cropsize, __func__, "array"); if(fits_read_subset(ifp, gal_fits_type_to_datatype(p->type), fpixel_i, lpixel_i, inc, p->bitnul, array, &anynul, &status)) gal_fits_io_error(status, NULL); /* If we have a floating point or double image, pixels with zero value should actually be a NaN. Unless the user specificly asks for it, make the conversion.*/ if(p->zeroisnotblank==0 && (p->type==GAL_TYPE_FLOAT32 || p->type==GAL_TYPE_FLOAT64) ) onecrop_zero_to_nan(array, cropsize, p->type); /* If a polygon is given, remove all the pixels within or outside of it.*/ if(p->polygon) { /* In WCS mode, crp->ipolygon was allocated and filled in wcspolygonflpixel (wcsmode.c). */ if(p->mode==IMGCROP_MODE_IMG) crp->ipolygon=p->ipolygon; polygonmask(crp, array, fpixel_i, lpixel_i[1]-fpixel_i[1]+1, lpixel_i[0]-fpixel_i[0]+1); if(p->mode==IMGCROP_MODE_WCS) free(crp->ipolygon); } /* Write the array into the image. */ status=0; if( fits_write_subset(ofp, gal_fits_type_to_datatype(p->type), fpixel_o, lpixel_o, array, &status) ) gal_fits_io_error(status, NULL); /* Write the selected region of this image as a string to include as a FITS keyword. Then we want to delete the last coma `,'.*/ j=0; for(i=0;i<ndim;++i) j += sprintf(®ion[j], "%ld:%ld,", fpixel_i[i], lpixel_i[i]); region[j-1]='\0'; /* A section has been added to the cropped image from this input image, so save the information of this image. */ sprintf(basename, "ICF%zu", crp->numimg); gal_fits_key_write_filename(basename, img->name, &headers); sprintf(regionkey, "%sPIX", basename); gal_fits_key_list_add_end(&headers, GAL_TYPE_STRING, regionkey, 0, region, 0, "Range of pixels used for " "this output.", 0, NULL); gal_fits_key_write(ofp, &headers); /* Free the allocated array. */ free(array); } else if(p->polygon && p->outpolygon==0 && p->mode==IMGCROP_MODE_WCS) free(crp->ipolygon); /* The crop is complete. */ return; } /*******************************************************************/ /****************** Check center *********************/ /*******************************************************************/ int onecrop_center_filled(struct onecropparams *crp) { struct cropparams *p=crp->p; void *array; size_t size, ndim, *dsize; fitsfile *ofp=crp->outfits; int status=0, anynul=0, type; long checkcenter=p->checkcenter; long naxes[2], fpixel[2], lpixel[2], inc[2]={1,1}; /* If checkcenter is zero, then don't check. */ if(checkcenter==0) return GAL_BLANK_UINT8; /* Get the final size of the output image. */ gal_fits_img_info(ofp, &type, &ndim, &dsize, NULL, NULL); naxes[0]=dsize[1]; naxes[1]=dsize[0]; /* Get the size and range of the central region to check. The +1 is because in FITS, counting begins from 1, not zero. It might happen that the image is actually smaller than the width to check the center (for example 1 or 2 pixels wide). In that case, we'll just use the full image to check. */ size = ( (naxes[0]>checkcenter ? checkcenter : naxes[0]) * (naxes[1]>checkcenter ? checkcenter : naxes[1]) ); fpixel[0] = naxes[0]>checkcenter ? (naxes[0]/2+1)-checkcenter/2 : 1; fpixel[1] = naxes[1]>checkcenter ? (naxes[1]/2+1)-checkcenter/2 : 1; lpixel[0] = naxes[0]>checkcenter ? (naxes[0]/2+1)+checkcenter/2 : naxes[0]; lpixel[1] = naxes[1]>checkcenter ? (naxes[1]/2+1)+checkcenter/2 : naxes[1]; /* For a check: printf("naxes: %ld, %ld\nfpixel: (%ld, %ld)\nlpixel: (%ld, %ld)\n" "size: %zu\n", naxes[0], naxes[1], fpixel[0], fpixel[1], lpixel[0], lpixel[1], size); */ /* Allocate the array and read in the pixels. */ array=gal_data_malloc_array(type, size, __func__, "array"); if( fits_read_subset(ofp, gal_fits_type_to_datatype(type), fpixel, lpixel, inc, p->bitnul, array, &anynul, &status) ) gal_fits_io_error(status, NULL); free(array); /* CFITSIO already checks if there are any blank pixels. If there are, then `anynul' will be 1, if there aren't it will be 0. So the output of this function is just the inverse of that number. */ return !anynul; } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/wcsmode.c���������������������������������������������������������������������0000644�0001750�0001750�00000046061�13216276304�013474� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <float.h> #include <string.h> #include <stdlib.h> #include <gnuastro/wcs.h> #include "main.h" #include "onecrop.h" /*******************************************************************/ /**************** Check for ui.c *********************/ /*******************************************************************/ /* This function is called from ui.c. Its job is to check the WCS values of this */ void wcsmode_check_prepare(struct cropparams *p, struct inputimgs *img) { double *pixscale; struct wcsprm *wcs=img->wcs; int i, status[4]={0,0,0,0}, ncorners=4; size_t *dsize=img->dsize, ndim=img->ndim; double imgcrd[8], phi[4], theta[4], pixcrd[8]; /* Check if the image is aligned with the WCS coordinates. Note that because of small floating point errors, some programs might still keep very small values in the off-diagonal matrix elements. */ if( fabs(wcs->pc[1]/wcs->pc[3])>1e-6 || fabs(wcs->pc[2]/wcs->pc[3])>1e-6 ) error(EXIT_FAILURE, 0, "%s: HDU %s: is not aligned to the " "celestial coordinates. The first FITS axis should be " "along the Right Ascension and the second FITS axis " "should be along the declination.\n\n" "Gnuastro's Warp program can align it with the following " "command:\n\n" " $ astwarp %s --hdu=%s --align\n", img->name, p->cp.hdu, img->name, p->cp.hdu); if(wcs->pc[0]>0) error(EXIT_FAILURE, 0, "%s: HDU %s: An increase in the first " "FITS axis pixel coordinates should be a decrease in the " "RA. You have to flip the image along the second axis " "before running Crop", img->name, p->cp.hdu); if(wcs->pc[3]<0) error(EXIT_FAILURE, 0, "%s: HDU %s: An increase in the second " "FITS axis pixel coordinates should translate to an " "increase in the declination. You have to flip the " "image along the first axis before running Crop", img->name, p->cp.hdu); /* Check the nature of the coordinates, currently we can only support RA and Dec, other modes haven't been checked. */ if( strcmp(wcs->ctype[0], "RA---TAN") || strcmp(wcs->ctype[1], "DEC--TAN") ) error(EXIT_FAILURE, 0, "currently the only WCS types usable are " "`RA---TAN' and `DEC--TAN' for the first and second axises " "respectively. The WCS types of `%s' (hdu %s) are `%s' and `%s' " "respectively", img->name, p->cp.hdu, wcs->ctype[0], wcs->ctype[1]); /* Check if the pixels are actually a square, then compare the resolution with the other input images. Due to floating point errors, some very small differences might exist in the pixel scale, so break out with an error only if the pixel scales are more different than 1e-6. */ pixscale=gal_wcs_pixel_scale(wcs); if( fabs(pixscale[0]-pixscale[1])/pixscale[0] > 1e-6 ) error(EXIT_FAILURE, 0, "%s: HDU %s: The pixel scale along " "the two image axises is not the same. The first axis " "is %.15g deg/pixel, while the second is %.15g", img->name, p->cp.hdu, pixscale[1], pixscale[0]); if(p->pixscale) { for(i=0;i<ndim;++i) if(p->pixscale[i] != pixscale[i]) error(EXIT_FAILURE, 0, "%s (hdu %s): has resolution of %g along " "dimension %d. However, previously checked input(s) had " "a resolution of %g in this dimension", img->name, p->cp.hdu, pixscale[i], i+1, p->pixscale[i]); free(pixscale); } else p->pixscale=pixscale; /* Set the coordinates of the dataset's corners. Note that `dsize' is in C order, while pixcrd is in FITS order.*/ pixcrd[0] = 1; pixcrd[1] = 1; pixcrd[2] = dsize[1]; pixcrd[3] = 1; pixcrd[4] = 1; pixcrd[5] = dsize[0]; pixcrd[6] = dsize[1]; pixcrd[7] = dsize[0]; /* Get the coordinates of the corners of the dataset in WCS. */ wcsp2s(wcs, ncorners, ndim, pixcrd, imgcrd, phi, theta, img->corners, status); /* Check if there was no error in the conversion. */ for(i=0;i<ncorners;++i) if(status[i]) error(EXIT_FAILURE, 0, "wcsp2s ERROR %d in row %d of pixcrd: %s", i, status[i], wcs_errmsg[status[i]]); /* Fill in the size of the dataset in WCS from the first pixel in the image. Note that `dsize' is in C axises, while the `pixscale', `corners' and `sized' are in FITS axises. */ img->sized[0] = ( img->dsize[1] * p->pixscale[0] / cos( img->corners[1] * M_PI / 180 ) ); img->sized[1] = img->dsize[0] * p->pixscale[1]; /* In case the image crosses the equator, we will calculate these values here so later on, we don't have to calculate them on every check. See the explanation above `point_in_dataset'. Note that in both 2D and 3D data, the declination is in the second coordinate (index 1). */ if( img->corners[1] * (img->corners[1]+img->sized[1]) < 0 ) { /* re in the comments above `point_in_dataset'. */ img->equatorcorr[0]=img->corners[0] -0.5*img->sized[0]*(1-cos(img->corners[1]*M_PI/180)); /* sre in the comments above `point_in_dataset'. */ img->equatorcorr[1]=img->sized[0]*cos(img->corners[1]*M_PI/180); } /* Just to check: printf("\n\n%s:\n", img->name); printf("(%.10f, %.10f)\n" "(%.10f, %.10f)\n" "(%.10f, %.10f)\n" "(%.10f, %.10f)\n\n", img->corners[0], img->corners[1], img->corners[2], img->corners[3], img->corners[4], img->corners[5], img->corners[6], img->corners[7]); exit(0); */ } /*******************************************************************/ /************ Check if WCS is in image **************/ /*******************************************************************/ /* Set the four sides around the point of interest in RA and Dec. NOTE: When the image is aligned with the celestial coordinates (current working paradigm), the declination is measured on a great circle, while the right ascension is not. So we have to consider this in calculating the difference in RA. */ void wcsmode_crop_corners(struct onecropparams *crp) { struct cropparams *p=crp->p; size_t i, ndim=p->imgs->ndim; double minra=FLT_MAX, mindec=FLT_MAX; double maxra=-FLT_MAX, maxdec=-FLT_MAX; double r, d, dr, h[MAXDIM], hr[MAXDIM]; size_t rmini=-1, rmaxi=-1, dmini=-1, dmaxi=-1; /* Set the four corners of the WCS region. */ if(p->polygon) { /* Find their minimum and maximum values. */ for(i=0;i<p->nvertices;++i) { if(p->wpolygon[i*2]>maxra) maxra=p->wpolygon[i*2]; if(p->wpolygon[i*2]<minra) minra=p->wpolygon[i*2]; if(p->wpolygon[i*2+1]>maxdec) maxdec=p->wpolygon[i*2+1]; if(p->wpolygon[i*2+1]<mindec) mindec=p->wpolygon[i*2+1]; } /* Set the corners: */ crp->corners[0] = maxra; crp->corners[1] = mindec; /* Bottom Left */ crp->corners[2] = minra; crp->corners[3] = mindec; /* Bottom Right */ crp->corners[4] = maxra; crp->corners[5] = maxdec; /* Top Left */ crp->corners[6] = minra; crp->corners[7] = maxdec; /* Top Right */ } else { /* Set the RA and Dec to use as center. */ r=crp->world[0]=p->centercoords[0][crp->out_ind]; d=crp->world[1]=p->centercoords[1][crp->out_ind]; /* Calculate the declination in radians for easy readability. */ dr=d*M_PI/180; /* Set the half width in each dimension. For the angular dimensions, also calculate it in radians. */ hr[0] = ( h[0] = ((double *)(p->width->array))[0] / 2 ) * M_PI / 180; hr[1] = ( h[1] = ((double *)(p->width->array))[1] / 2 ) * M_PI / 180; /* Set the corners of this crop. */ crp->corners[0] = r+h[0]/cos(dr-hr[1]); crp->corners[1] = d-h[1]; /* Bottom left. */ crp->corners[2] = r-h[0]/cos(dr-hr[1]); crp->corners[3] = d-h[1]; /* Bottom Right. */ crp->corners[4] = r+h[0]/cos(dr+hr[1]); crp->corners[5] = d+h[1]; /* Top Left. */ crp->corners[6] = r-h[0]/cos(dr+hr[1]); crp->corners[7] = d+h[1]; /* Top Right. */ } /* Set the bottom width and height of the crop in degrees. Note that the width changes as the height changes, so here we want the height and the lowest declination. Note that in 2D on the bottom edge, corners[0] is the maximum RA and corners[2] is the minimum RA. For all the 2D region, corners[5] is one of the maximum declinations and corners[1] is one of the the minimum declinations. North and south hemispheres are no problem: When using the center, they are set properly (in any hemisphere) and for a polygon, the minimums and maximums are automatically found. */ rmini = ndim; /* First element in second corner. */ rmaxi = 0; /* First element. */ dmini = 1; /* Second element. */ dmaxi = 5; /* Second element in third corner. */ crp->sized[0]=( (crp->corners[rmaxi]-crp->corners[rmini]) / cos(crp->corners[dmini]*M_PI/180) ); crp->sized[1]=crp->corners[dmaxi]-crp->corners[dmini]; /* In case the crop crosses the equator, then we need these two corrections. See the complete explanations above `point_in_dataset'. */ if(crp->corners[1]*(crp->corners[1]+crp->sized[1]) < 0 ) { /* re in the explanations above `point_in_dataset'. */ crp->equatorcorr[0]=crp->corners[0] -0.5*crp->sized[0]*(1-cos(crp->corners[1]*M_PI/180)); /* sre in the explanations above `point_in_dataset'. */ crp->equatorcorr[1]=crp->sized[0]*cos(crp->corners[1]*M_PI/180); } /* Just to check: printf("\n\n%g, %g:\n", r, d); printf("\t(%.10f, %.10f)\n" "\t(%.10f, %.10f)\n" "\t(%.10f, %.10f)\n" "\t(%.10f, %.10f)\n\n", crp->corners[0], crp->corners[1], crp->corners[2], crp->corners[3], crp->corners[4], crp->corners[5], crp->corners[6], crp->corners[7]); exit(0); */ } /* We have the polygon vertices in WCS coordinates and need to change them to one input image's pixel coordinates. */ void fillcrpipolygon(struct onecropparams *crp) { struct cropparams *p=crp->p; gal_data_t *tmp, *coords=NULL; size_t i, d, ndim=p->imgs->ndim; /* Allocate the necessary arrays for each column. */ for(d=0;d<ndim;++d) gal_list_data_add_alloc(&coords, NULL, GAL_TYPE_FLOAT64, 1, &p->nvertices, NULL, 0, -1, NULL, NULL, NULL); /* Fill in the world coordinate columns. */ for(i=0;i<p->nvertices;++i) { d=0; for(tmp=coords;tmp!=NULL;tmp=tmp->next) ((double *)(tmp->array))[i] = p->wpolygon[ i * ndim + d++ ]; } /* Convert them to image coordinates. */ gal_wcs_world_to_img(coords, p->imgs[crp->in_ind].wcs, 1); /* Allocate the image polygon array, and put the image polygon vertice values into it. */ crp->ipolygon=gal_data_malloc_array(GAL_TYPE_FLOAT64, ndim*p->nvertices, __func__, "crp->ipolygon"); for(i=0;i<p->nvertices;++i) { d=0; for(tmp=coords;tmp!=NULL;tmp=tmp->next) crp->ipolygon[ i * ndim + d++ ] = ((double *)(tmp->array))[i]; } /* Clean up. */ gal_list_data_free(coords); } /* BASICS: ======= An image is a rectangle, but the sky is on a globe. When the images are aligned to the celstial coordinates, (as we have required here in wcscheckprepare) the first FITS axis shows change in RA, while the second axis shows change in Dec. The declination always changes along a great circle, so there is no problem. But unless declination is constrained to zero, RA changes on small circles. See the rectangle below, assume it is an image. To check if a given point is within the same declination as this rectangle is very simple, since d3==d4 and d1==d2. Note that r1>r2 and r3>r4 (because right ascension increases to the east). (r3,d3) ------------------ (r4,d4) | | | | | | | | (r1,d1) ------------------ (r2,d2) But for RA, the same number of pixels on each declination, corresponds to different ranges in right ascention. As the declination gets higher in the northern hemisphere (where the declination rises towards the top of the image) r1-r2 becomes smaller than r3-r4. So, in terms of coverage in RA and Dec, this box should rather be shown like this trapezoid (exaggerated): -------------------- | | | | (Northern hemisphere) | | | | -------------- On the southern hemisphere it should be shown like this: ---------------- | | | | (Southern hemisphere) | | | | ---------------------- The functional form of the change is the inverse cosine, so: (r3-r4)=(r1-r2)/cos(d3-d1) (North) (r1-r2)=(r3-r4)/cos(d1-d3) (South) QUESTION: ======== Is a given point at the RA and Dec of (rp,dp) inside our rectangular image? IMAGE IS FULLY WITHIN ONE HEMISPHERE ------------------------------------ Our reference point for the image is the first pixel in the image, which by convention is the (r1,d1) point in the rectangle above. We also have the angular size of the rectangular image as 'sr', 'sd' (for "size in RA" and "size in dec"). NOTE: This has to be We also assume r1+sr and d1+sd are the distances to the last pixels in our rectangular image. As explained above, to check the declination range, everything is very easy: dp>=d1 && dp<=d1+sd For RA, things become a little more complicated (recall that r1>r3). `n` is defined as half of the extra space between the top and bottom lines of the two trapezoids. (North) n=0.5*sr*(1/cos(dp-d1)-1) ==> rp<=r1+n && rp>=r1-sr-n (South) n=0.5*sr*(1-cos(dp-d1)) ==> rp<=r1-n && rp>=r1-sr+n IMAGE CROSSES THE EQUATOR ------------------------- When d1*(d1+sd)<0, the image crosses the equator (d1 is negative and d1+sd is positive). In this case, we define `re` and `sre` as an equivalent of r1 and sr but on the equator: re=r1-0.5*sr*(1-cos(d1)) && sre=sr*cos(d1) then for all the points with negative declination we use the (South) equations of above as before and for those points that have a positive declination, we use the North formula but replacing r1 with re, d1 with 0 and sr with sre. INPUTS ------ p[]: Point coordinates (rp and dp above). i[]: Coordinates of first pixel in image. (r1 and d1 above). s[]: Size/width of box (sr and sd above). c[]: Corrections if equator is passed, (se and sre above). IMPORTANT: It is assumed that the dimensions are ordered with: 0: RA 1: Dec 2: Third dimension (independent of RA and Dec). */ static int point_in_dataset(double *p, double *i, double *s, double *c, size_t ndim) { double n; /* In the RA and Dec checks, first check the declination. If it is not in range, you can safely return 0. */ if(p[1]>=i[1] && p[1]<=i[1]+s[1]) { if(p[1]<=0) /* Point is in southern hemisphere, it */ { /* doesn't matter if image passes equator! */ n=0.5f*s[0]*( 1 - cos((p[1]-i[1])*M_PI/180) ); if(p[0]<=i[0]-n && p[0]>=i[0]-s[0]+n) return 1; } else /* Point is in the northern hemisphere. */ { if( i[1] * (s[1]+i[1]) > 0 ) /* Image does not cross equator. */ { n=0.5f*s[0]*( 1/cos((p[1]-i[1])*M_PI/180) - 1); if(p[0]<=i[0]+n && p[0]>=i[0]-s[0]-n) return 1; } else /* Image crosses the equator.*/ { n=0.5f*c[1]*( 1/cos((p[1] )*M_PI/180) - 1); if(p[0]<=c[0]+n && p[0]>=c[0]-c[1]-n) return 1; } } } return 0; } /* Is there an overlap between this crop box and the survey image? This function will return 0 if there isn't and 1 if there is. We don't want to necessarily assume that the crop box is smaller than the survey images. If we made that assumption, we only had to check if the corners of the crop are in the image. When we allow the input survey images to be smaller than the crop box, it might happen that none of the corners of the crop are in the image but there is an overlap (the survey image is completely within the crop box). So we have to check both. */ int wcsmode_overlap(struct onecropparams *crp) { double *d, *fd; double *i, *s, *c; /* for clear viewing. */ struct cropparams *p=crp->p; size_t ndim=crp->p->imgs->ndim; /* First check if the corners of the crop are in the image.*/ s=p->imgs[crp->in_ind].sized; i=p->imgs[crp->in_ind].corners; c=p->imgs[crp->in_ind].equatorcorr; fd=(d=crp->corners) + 8; do { /* As long as one of the crop corners are in the image, we know there is overlap and can return a true value. We don't need to check all corners. */ if( point_in_dataset(d, i, s, c, ndim) ) return 1; d+=ndim; } while(d<fd); /* None of the crop box corners where within the image. Now check if the image corners are within the crop.*/ s=crp->sized; i=crp->corners; c=crp->equatorcorr; fd=(d=p->imgs[crp->in_ind].corners) + 8; do { if( point_in_dataset(d, i, s, c, ndim) ) return 1; d+=ndim; } while(d<fd); /* If control reaches here, there was no overlap. */ return 0; } �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/crop.c������������������������������������������������������������������������0000644�0001750�0001750�00000032241�13216276304�012771� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <unistd.h> #include <string.h> #include <stdlib.h> #include <gnuastro/fits.h> #include <gnuastro/threads.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "onecrop.h" #include "wcsmode.h" /* Write the log entry for each crop. A maximum length of FILENAME_BUFFER_IN_VERB characters is set for the filename to be displayed in stdout in verbose mode. This length is set to make the output on the user's terminal reasonable (in one line). So when the filename is longer than this, its first set of characters are truncated. In the log-file there is no truncation, therefore the log file should be used for checking the outputs, not the outputs printed on the screen. */ static void crop_verbose_info(struct onecropparams *crp) { char *filestatus, *msg; size_t outnamelen=strlen(crp->name);; /* Human readable values. */ filestatus = ( crp->centerfilled==0 ? ( crp->numimg == 0 ? "no overlap" : "removed (blank center)" ) : "created"); /* Define the output string based on the length of the output file. */ if ( outnamelen > FILENAME_BUFFER_IN_VERB ) asprintf(&msg, "...%s %s: %zu input%s.", &crp->name[ outnamelen - FILENAME_BUFFER_IN_VERB + 3 ], filestatus, crp->numimg, crp->numimg==1 ? "" :"s"); else asprintf(&msg, "%-*s %s: %zu input%s.", FILENAME_BUFFER_IN_VERB, crp->name, filestatus, crp->numimg, crp->numimg==1 ? "" : "s"); /* Print the results. */ gal_timing_report(NULL, msg, 2); free(msg); } /* Print final statistics in verbose mode. */ static void crop_verbose_final(struct cropparams *p) { char *msg; gal_data_t *tmp; size_t i, counter=0, numcrops=0, numstitched=0, numcfilled=0; /* This function is only useful in verbose (non-quiet) mode. */ if(p->cp.quiet) return; /* The information is only available if the user asks for a log file. */ if(p->catname && p->log) { /* Get the basic counts. */ for(tmp=p->log; tmp!=NULL; tmp=tmp->next) switch(++counter) { case 2: for(i=0;i<p->numout;++i) if( ((unsigned short *)(tmp->array))[i] > 1) ++numstitched; break; case 3: /* When the center wasn't checked it has a value of -1, and when it was checked and the center was filled, it has a value of 1. So if `array[i]==0', we know that the file was removed. */ for(i=0;i<p->numout;++i) { if( ((unsigned char *)(tmp->array))[i] ) ++numcrops; if( ((unsigned char *)(tmp->array))[i] == 1 ) ++numcfilled; } break; } /* Print the basic information. */ asprintf(&msg, "%zu crops created.", numcrops); gal_timing_report(NULL, msg, 1); free(msg); /* Only if the user wanted to check the center. */ if(p->checkcenter) { asprintf(&msg, "%zu filled in the center.", numcfilled); gal_timing_report(NULL, msg, 1); free(msg); } /* Only if there were stitched images. */ if(numstitched) { asprintf(&msg, "%zu crops used more than one input.", numstitched); gal_timing_report(NULL, msg, 1); free(msg); } } } static void crop_write_to_log(struct onecropparams *crp) { char **strarr; gal_data_t *tmp; size_t counter=0; for(tmp=crp->p->log; tmp!=NULL; tmp=tmp->next) { switch(++counter) { case 1: strarr=tmp->array; gal_checkset_allocate_copy(crp->name, &strarr[crp->out_ind]); break; case 2: ((unsigned short *)(tmp->array))[crp->out_ind]=crp->numimg; break; case 3: ((unsigned char *)(tmp->array))[crp->out_ind]=crp->centerfilled; break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to fix " "the problem. The value of %zu is not valid for `counter'", __func__, PACKAGE_BUGREPORT, counter); } } } static void * crop_mode_img(void *inparam) { struct onecropparams *crp=(struct onecropparams *)inparam; struct cropparams *p=crp->p; size_t i; int status; struct inputimgs *img; /* In image mode, we always only have one image. */ crp->in_ind=0; /* The whole catalog is from one image, so you can get the information here:*/ img=&p->imgs[crp->in_ind]; crp->infits=gal_fits_hdu_open_format(img->name, p->cp.hdu, 0); /* Go over all the outputs that are assigned to this thread: */ for(i=0; crp->indexs[i]!=GAL_BLANK_SIZE_T; ++i) { /* Set all the output parameters: */ crp->out_ind=crp->indexs[i]; crp->outfits=NULL; crp->numimg=1; /* In Image mode there is only one input image. */ onecrop_name(crp); /* Crop the image. */ onecrop(crp); /* Check the final output: */ if(crp->numimg) { /* Check if the center of the crop is filled or not. */ crp->centerfilled=onecrop_center_filled(crp); /* Add the final headers and close output FITS image: */ gal_fits_key_write_version(crp->outfits, NULL, PROGRAM_NAME); status=0; if( fits_close_file(crp->outfits, &status) ) gal_fits_io_error(status, "CFITSIO could not close " "the opened file"); /* Remove the output image if its center was not filled. */ if(crp->centerfilled==0) { errno=0; if(unlink(crp->name)) error(EXIT_FAILURE, errno, "can't delete %s (center" "was blank)", crp->name); } } else crp->centerfilled=0; /* Report the status on stdout if verbose mode is requested. */ if(!p->cp.quiet) crop_verbose_info(crp); if(p->cp.log) crop_write_to_log(crp); } /* Close the input image. */ status=0; if( fits_close_file(crp->infits, &status) ) gal_fits_io_error(status, "could not close FITS file"); /* Wait until all other threads finish. */ if(p->cp.numthreads>1) pthread_barrier_wait(crp->b); return NULL; } static void * crop_mode_wcs(void *inparam) { struct onecropparams *crp=(struct onecropparams *)inparam; struct cropparams *p=crp->p; size_t i; int status; /* Go over all the output objects for this thread. */ for(i=0; crp->indexs[i]!=GAL_BLANK_SIZE_T; ++i) { /* Set all the output parameters: */ crp->out_ind=crp->indexs[i]; crp->outfits=NULL; crp->name=NULL; crp->numimg=0; /* Set the sides of the crop in RA and Dec */ wcsmode_crop_corners(crp); /* Go over all the images to see if this target is within their range or not. */ crp->in_ind=0; do if(wcsmode_overlap(crp)) { /* Open the input FITS file. */ crp->infits=gal_fits_hdu_open_format(p->imgs[crp->in_ind].name, p->cp.hdu, 0); /* If a name isn't set yet, set it. */ if(crp->name==NULL) onecrop_name(crp); /* Increment the number of images used (necessary for the header keywords that are written in `onecrop'). Then do the crop. */ ++crp->numimg; onecrop(crp); /* Close the file. */ status=0; if( fits_close_file(crp->infits, &status) ) gal_fits_io_error(status, "could not close FITS file"); } while ( ++(crp->in_ind) < p->numin ); /* Correct in_ind. The loop above went until `in_ind' is one more than the index for the last input image (that is how it exited the loop). But `crp->in_ind' is needed later, so correct it here. */ --crp->in_ind; /* Check the final output: */ if(crp->numimg) { /* See if the center is filled. */ crp->centerfilled=onecrop_center_filled(crp); /* Write all the dependency versions and close the file. */ gal_fits_key_write_version(crp->outfits, NULL, PROGRAM_NAME); status=0; if( fits_close_file(crp->outfits, &status) ) gal_fits_io_error(status, "CFITSIO could not close the " "opened file"); if(crp->centerfilled==0) { errno=0; if(unlink(crp->name)) error(EXIT_FAILURE, errno, "%s", crp->name); } } else { onecrop_name(crp); crp->centerfilled=0; } /* Report the status on stdout if verbose mode is requested. */ if(!p->cp.quiet) crop_verbose_info(crp); if(p->cp.log) crop_write_to_log(crp); } /* Wait until all other threads finish, then return. */ if(p->cp.numthreads>1) pthread_barrier_wait(crp->b); return NULL; } /*******************************************************************/ /************** Output function ****************/ /*******************************************************************/ /* Main function for the Image Mode. It is assumed that if only one crop box from each input image is desired, the first and last pixels are already set, irrespective of how the user specified that box. */ void crop(struct cropparams *p) { int err=0; char *tmp; pthread_t t; /* We don't use the thread id, so all are saved here. */ pthread_attr_t attr; pthread_barrier_t b; struct onecropparams *crp; size_t i, *indexs, thrdcols; gal_list_str_t *comments=NULL; size_t nt=p->cp.numthreads, nb; void *(*modefunction)(void *)=NULL; /* Set the function to run: */ modefunction = p->mode==IMGCROP_MODE_IMG ? &crop_mode_img : &crop_mode_wcs; /* Allocate the array of structures to keep the thread and parameters for each thread. */ errno=0; crp=malloc(nt*sizeof *crp); if(crp==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `crp'", __func__, nt*sizeof *crp); /* Distribute the indexs into the threads (this is needed even if we only have one object where p->cs0 is not defined): */ gal_threads_dist_in_threads(p->catname ? p->numout : 1, nt, &indexs, &thrdcols); /* Run the job, if there is only one thread, don't go through the trouble of spinning off a thread! */ if(nt==1) { crp[0].p=p; crp[0].indexs=indexs; modefunction(&crp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if(p->numout<nt) nb=p->numout+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Spin off the threads: */ for(i=0;i<nt;++i) if(indexs[i*thrdcols]!=GAL_BLANK_SIZE_T) { crp[i].p=p; crp[i].b=&b; crp[i].indexs=&indexs[i*thrdcols]; err=pthread_create(&t, &attr, modefunction, &crp[i]); if(err) error(EXIT_FAILURE, 0, "%s: can't create thread %zu", __func__, i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } /* Print the log file. */ if(p->cp.log) { if(p->checkcenter) { asprintf(&tmp, "Width of central check box: %zu", p->checkcenter); gal_list_str_add(&comments, tmp, 0); } gal_checkset_writable_remove(LOGFILENAME, 0, p->cp.dontdelete); gal_table_write_log(p->log, PROGRAM_STRING, &p->rawtime, comments, LOGFILENAME, p->cp.quiet); gal_list_str_free(comments, 1); } /* Print the final verbose info, save log, and clean up: */ crop_verbose_final(p); free(indexs); free(crp); } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/ui.c��������������������������������������������������������������������������0000644�0001750�0001750�00000100522�13216276304�012441� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/wcs.h> #include <gnuastro/list.h> #include <gnuastro/fits.h> #include <gnuastro/blank.h> #include <gnuastro/table.h> #include <gnuastro/dimension.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/tableintern.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "onecrop.h" #include "wcsmode.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "[Crop-identifiers] ASTRdata ..."; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will create cutouts, " "thumbnails, postage stamps or crops of region(s) from input image(s) " "using image or celestial coordinates. If muliple crops are desired, a " "catalog must be provided. When in WCS mode, if the cut out covers more " "than one input image, all overlapping input images will be stitched in " "the output.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct cropparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->poptions = program_options; cp->numthreads = gal_threads_number(); cp->coptions = gal_commonopts_options; /* Initalize necessary parameters. */ p->mode = IMGCROP_MODE_INVALID; cp->searchin = GAL_TABLE_SEARCH_INVALID; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; cp->coptions[i].doc="Extension name or number of (all) input(s)."; break; case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: cp->coptions[i].group=UI_GROUP_CENTER_CATALOG; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct cropparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: gal_list_str_add(&p->inputs, arg, 0); ++p->numin; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /* Parse the mode to interpret the given coordinates. */ void * ui_parse_coordinate_mode(struct argp_option *option, char *arg, char *filename, size_t lineno, void *junk) { char *outstr; /* We want to print the stored values. */ if(lineno==-1) { gal_checkset_allocate_copy( *(int *)(option->value)==IMGCROP_MODE_IMG ? "img" : "wcs", &outstr ); return outstr; } else { if (!strcmp(arg, "img")) *(int *)(option->value)=IMGCROP_MODE_IMG; else if (!strcmp(arg, "wcs")) *(int *)(option->value)=IMGCROP_MODE_WCS; else error_at_line(EXIT_FAILURE, 0, filename, lineno, "`%s' (value to " "`--mode') not recognized as an input mode. " "Recognized values are `img' and `wcs'. This option " "is necessary to identify the nature of your input " "coordinates.\n\n" "Please run the following command for more " "information (press the `SPACE' key to go down and " "`q' to return to the command-line):\n\n" " $ info gnuastro \"Crop modes\"\n", arg); return NULL; } } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct cropparams *p) { double *darray; int i, checksum; /* Make sure that only one of the crop definitions is given. */ checksum = ( (p->center!=NULL) + (p->catname!=NULL) + (p->section!=NULL) + (p->polygon!=NULL) ); switch(checksum) { case 0: error(EXIT_FAILURE, 0, "no crop definition. You can use any of the " "following options to define the crop(s): `--center', " "`--catalog', `--section', or `--polygon'. Please run this " "command for more information:\n\n" " $ info gnuastro \"Crop modes\"\n"); case 1: /* Everything is ok, just ignore the switch structure. */ break; default: error(EXIT_FAILURE, 0, "more than one crop type specified. In each " "run, only one crop definition is acceptable on the " "command-line or in configuration files. You have called: " "%s%s%s%s\b\b.", p->center!=NULL ? "`--center', " : "", p->catname!=NULL ? "`--catalog', " : "", p->section!=NULL ? "`--section', " : "", p->polygon!=NULL ? "`--polygon', " : ""); } /* The width values must not be negative. */ if(p->width) { darray=p->width->array; for(i=0;i<p->width->size;++i) if(darray[i]<=0.0f) error(EXIT_FAILURE, 0, "%g is <=0. The values to the `--width' " "option must be larger than zero. %g is input number %d to " "this option", darray[i], darray[i], i+1); } /* Section is currentlyl only defined in Image mode. */ if(p->section && p->mode!=IMGCROP_MODE_IMG) error(EXIT_FAILURE, 0, "The `--section' option is only available in " "image coordinate mode, currently it doesn't work with WCS mode. " "Please run with `--mode=img' and if necessary, change the " "values accordingly"); /* Sanity checks and mode setting based on the desired crop. */ if(p->catname) { /* If the searchin option has been given. */ if(p->cp.searchin==GAL_TABLE_SEARCH_INVALID) error(EXIT_FAILURE, 0, "%s: no field specified to search for " "columns. Please use the `--searchin' option to specify " "which column meta-data you would like to search in: `name', " "`unit' and `comment'. You may also select columns by their " "number, which won't use this option, but for complentess its " "best for this option to have a value", p->catname); /* If it is a FITS file, we need the HDU. */ if( gal_fits_name_is_fits(p->catname) && p->cathdu==NULL ) error(EXIT_FAILURE, 0, "%s: no hdu given. Please use the `--cathdu' " "option to specify which extension contains the table", p->catname); /* Atleast one of the (X,Y), and (RA,Dec) set of columns are necessary. Note that we have checked that they are together if given, so we only need to check one of the two in each couple. */ if(p->coordcol==NULL) error(EXIT_FAILURE, 0, "no crop center columns given to read from " "the input catalog (`%s'). Please use `--coordcol' two times " "to specify the column keeping the center position the " "respective dimension.\n\n" "For more information on how to select columns in Gnuastro, " "please run the following command:\n\n" " $ info gnuastro \"Selecting table columns\"", p->catname); } /* Parse the polygon vertices if they are given to make sure that it is in the proper format. */ if(p->polygon) { onecrop_parse_polygon(p); if(p->nvertices<3) error(EXIT_FAILURE, 0, "a polygon has to have 3 or more vertices, " "you have only given %zu (%s)", p->nvertices, p->polygon); if(p->outpolygon && p->numin>1) error(EXIT_FAILURE, 0, "currently in WCS mode, outpolygon can only " "be set to zero when there is one image, you have given %zu " "images. For multiple images the region will be very large. " "It is best if you first crop out the larger region you want " "into one image, then mask the polygon", p->numin); } else p->wpolygon=p->ipolygon=NULL; /* If we are in WCS mode, noblanks must be off */ if(p->mode==IMGCROP_MODE_WCS && p->noblank) error(EXIT_FAILURE, 0, "`--noblanks` (`-b`) is only for image mode. " "You have called it with WCS mode"); } static void ui_check_options_and_arguments(struct cropparams *p) { /* Make sure we actually have inputs. */ if(p->inputs==NULL) error(EXIT_FAILURE, 0, "no input file given"); /* Make sure that a HDU is also given. */ if(p->cp.hdu==NULL ) error(EXIT_FAILURE, 0, "no HDU specified. When the input is a FITS " "file, a HDU must also be specified, you can use the `--hdu' " "(`-h') option and give it the HDU number (starting from " "zero), extension name, or anything acceptable by CFITSIO"); /* If in image mode, there should only be one input image. */ if(p->mode==IMGCROP_MODE_IMG && p->numin>1) error(EXIT_FAILURE, 0, "in image mode, only one input image may be " "specified"); /* If no output name is given, set it to the current directory. */ if(p->cp.output==NULL) gal_checkset_allocate_copy("./", &p->cp.output); /* Only catalog mode needs multiple threads and a directory for the output. */ if(p->catname) { /* When multiple threads need to access a file, CFITSIO needs to be configured with the `--enable-reentrant` option. */ if(p->cp.numthreads>1 && fits_is_reentrant()==0) error(EXIT_FAILURE, 0, "CFITSIO was not configured with the " "`--enable-reentrant` option but you have asked to crop " "on %zu threads.\n\nPlease configure, make and install CFITSIO " "again with this flag. Alternatively, to avoid this error " "you can set the number of threads to 1 by adding the " "`--numthreads=1` or `-N1` options. Please run the following " "command to learn more about configuring CFITSIO:\n\n" " $ info gnuastro CFITSIO", p->cp.numthreads); /* Make sure the given output is a directory. */ gal_checkset_check_dir_write_add_slash(&p->cp.output); } else { p->cp.numthreads=1; p->outnameisfile=gal_checkset_dir_0_file_1(p->cp.output, p->cp.dontdelete); } } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ /* When the crop is defined by its center, the final width that we need must be in actual number of pixels (an integer). But the user's values can be in WCS mode or even in image mode, they may be non-integers. */ static void ui_set_iwidth(struct cropparams *p) { gal_data_t *newwidth; double pwidth, *warray; size_t i, ndim=p->imgs->ndim; /* Make sure a width value is actually given. */ if(p->width==NULL) error(EXIT_FAILURE, 0, "no crop width specified. When crops are " "defined by their center (with `--center' or `--catalog') a " "width is necessary (using the `--width' option)"); /* Make sure that the width array only has one element or the same number of elements as the input's dimensions. */ if(p->width->size!=ndim && p->width->size!=1) error(EXIT_FAILURE, 0, "%zu values give to `--width', but input is %zu " "dimensions. It can only take either one value (same width in all " "dimensions), or the same number as the input's dimensions", p->width->size, ndim); /* If the width array has only one value, that single value should be used for all dimensions. */ if(p->width->size==1) { /* Allocate the new width dataset. */ newwidth=gal_data_alloc(NULL, p->width->type, 1, &ndim, NULL, 0, -1, NULL, NULL, NULL); /* Fill the new width. */ warray=newwidth->array; for(i=0;i<ndim;++i) warray[i] = *(double *)(p->width->array); /* Free the old (single element) width dataset and put the new one in its place. */ gal_data_free(p->width); p->width=newwidth; } else warray=p->width->array; /* Fill in `p->iwidth' depending on the mode. */ for(i=0;i<ndim;++i) { /* Set iwidth. */ if(p->mode==IMGCROP_MODE_WCS) { /* Convert the width in units of the input's WCS into pixels. */ pwidth = warray[i]/p->pixscale[i]; if(pwidth<3 || pwidth>50000) error(EXIT_FAILURE, 0, "%g (width along dimension %zu) " "translates to %.0f pixels. This is probably not what " "you wanted. Note that the resolution in this dimension " "is %g", warray[i], i+1, pwidth, p->pixscale[i]); /* Write the single valued width in WCS and the image width for this dimension. */ p->iwidth[i]=GAL_DIMENSION_FLT_TO_INT(pwidth); if(p->iwidth[i]%2==0) { p->iwidth[i] += 1; warray[i] += p->pixscale[i]; } } else { p->iwidth[i]=GAL_DIMENSION_FLT_TO_INT(warray[i]); if(p->iwidth[i]%2==0) p->iwidth[i] += 1; } } /* For a check: printf("Width: "); for(i=0;i<ndim;++i) printf("\t%ld\n\t", p->iwidth[i]); exit(0); */ } static void ui_read_cols(struct cropparams *p) { char colname[100]; gal_data_t *cols, *tmp, *corrtype=NULL; gal_list_str_t *colstrs=NULL, *extracolstr, *lastcolstr; size_t i, ncoordcols, counter=0, dcounter=0, ndim=p->imgs->ndim; /* See if the number of columns given for coordinates corresponds to the number of dimensions of the input dataset. */ if(p->coordcol) { /* Check if the number of columns given for coordinates is the same as the number of dimensions in the input dataset(s). */ ncoordcols=gal_list_str_number(p->coordcol); if( ncoordcols < ndim) error(EXIT_FAILURE, 0, "`--coordcol' was called %zu times, but the " "input dataset%s %zu dimensions. Recall that through " "`--coordcol' you are specifying the columns containing the " "coordinates of the center of the crop in a catalog", ncoordcols, (p->numin==1?" has":"s have"), ndim); /* If the number of given columns is more than the input's dimensions, then we'll just delete all the unnecessary columns. */ else if( ncoordcols > ndim ) { /* Go over the columns find the last, but first initialize the two (`lastcolstr' to avoid compiler warnings). */ lastcolstr=extracolstr=p->coordcol; for(i=0;i<ndim;++i) { /* Keep the last node if on the last (useful) column. */ if(i==ndim-1) lastcolstr=extracolstr; /* Go onto the next one. */ extracolstr=extracolstr->next; } /* Set the `next' element of the last node to NULL and free the extra ones. */ lastcolstr->next=NULL; gal_list_str_free(extracolstr, 1); } } else error(EXIT_FAILURE, 0, "no coordinate columns specified. When a catalog" "is given, it is necessary to identify which columns identify " "the coordinate values in which dimension.\n\n" "You can do this by calling `--coordcol' multiple times, the " "order must be in the same order as the input's dimensions. " "For more information on how to select columns in Gnuastro, " "please run the following command:\n\n" " $ info gnuastro \"Selecting table columns\""); /* If a name column was also given, the put that as the first column to read, otherwise just use the given set of columns (in the same order). */ if(p->namecol) { gal_list_str_add(&colstrs, p->namecol, 0); colstrs->next=p->coordcol; } else colstrs=p->coordcol; /* Read the desired columns from the file. */ cols=gal_table_read(p->catname, p->cathdu, colstrs, p->cp.searchin, p->cp.ignorecase, p->cp.minmapsize, NULL); /* Set the number of objects (rows in each column). */ p->numout=cols->size; /* Make sure more columns were not read (the name matchings might result in more than one column being read from the inputs). */ if( gal_list_data_number(cols) != ndim + (p->namecol!=NULL) ) gal_tableintern_error_col_selection(p->catname, p->cathdu, "too many " "columns were selected by the given " "values to the options ending in " "`col'."); /* Put the information in each column in the proper place. */ while(cols!=NULL) { /* Pop out the top node. */ tmp=gal_list_data_pop(&cols); /* See which column it is. */ switch(++counter) { case 1: if(p->namecol) { sprintf(colname, "crop name prefix"); corrtype = (tmp->type==GAL_TYPE_STRING ? tmp : gal_data_copy_to_new_type_free(tmp, GAL_TYPE_STRING)); p->name=corrtype->array; } else { sprintf(colname, "position in dimension %zu", dcounter+1); corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT64); p->centercoords[ dcounter++ ]=corrtype->array; } break; default: sprintf(colname, "position in dimension %zu", dcounter+1); corrtype=gal_data_copy_to_new_type_free(tmp, GAL_TYPE_FLOAT64); p->centercoords[ dcounter++ ] = corrtype->array; } /* Sanity check and clean up. Note that it might happen that the input structure is already freed. In that case, `corrtype' will be NULL. */ if(corrtype) { /* Make sure there are no blank values in this column. */ if( gal_blank_present(corrtype, 1) ) error(EXIT_FAILURE, 0, "%s: column with %s has blank values. " "Input columns must not contain blank values", gal_fits_name_save_as_string(p->catname, p->cathdu), colname); /* Free the unnecessary sturcture information. The correct-type (`corrtype') data structure's array is necessary for later steps, so its pointer has been copied in the main program's structure. Hence, we should set the structure's pointer to NULL so the important data isn't freed.*/ corrtype->array=NULL; gal_data_free(corrtype); corrtype=NULL; } } } static void ui_prepare_center(struct cropparams *p) { double *carray; size_t i, ndim=p->imgs->ndim; /* Allocate space to keep the central positions. */ errno=0; p->centercoords=malloc(ndim*sizeof *p->centercoords); if( p->centercoords==NULL ) error(EXIT_FAILURE, 0, "%s: %zu bytes for `p->centercoords'", __func__, ndim*sizeof *p->centercoords); /* Set the integer widths of the crop(s) when defined by center. */ ui_set_iwidth(p); /* For a catalog, we have a separate function, but for a single center value, put the center values into an array. This will essentially simulate a catalog with one row. So from this point on, there is no difference between a catalog input and a central position input. */ if(p->catname) ui_read_cols(p); else { carray=p->center->array; for(i=0;i<ndim;++i) { p->centercoords[i]=gal_data_malloc_array(GAL_TYPE_FLOAT64, 1, __func__, "p->centercoords[i]"); p->centercoords[i][0]=carray[i]; } } } /* Add all the columns of the log file. Just note that since this is a linked list, we have to add them in the opposite order. */ static void ui_make_log(struct cropparams *p) { char *comment; /* Return if no long file was requested. */ if(p->cp.log==0) return; /* Column to specify if the central pixels are filled. */ asprintf(&comment, "Are the central pixels filled? (1: yes, 0: no, " "%u: not checked)", GAL_BLANK_UINT8); gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_UINT8, 1, &p->numout, NULL, 1, p->cp.minmapsize, "CENTER_FILLED", "bool", comment); free(comment); /* Column for number of datasets used in this crop. */ gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_UINT16, 1, &p->numout, NULL, 1, p->cp.minmapsize, "NUM_INPUTS", "count", "Number of input datasets used to make this crop."); /* Filename of crop. */ gal_list_data_add_alloc(&p->log, NULL, GAL_TYPE_STRING, 1, &p->numout, NULL, 1, p->cp.minmapsize, "CROP_NAME", "name", "File name of crop."); } void ui_preparations(struct cropparams *p) { fitsfile *tmpfits; struct inputimgs *img; int status, firsttype=0; size_t input_counter, firstndim=0; /* For polygon and section, there should be no center checking. */ if(p->polygon || p->section) p->checkcenter=0; /* Allocate space for all the input images. This is done here because WCSLIB is unfortunately not thread-safe when reading the WCS information from the FITS files. In cases where the number of cropped images are more than the input images, this can also be a preformance boost because each image information is only read once. The images are filled in opposite order because we used a linked list to read them in, which is a first in first out structure.*/ errno=0; p->imgs=malloc(p->numin*sizeof *p->imgs); if(p->imgs==NULL) error(EXIT_FAILURE, errno, "%s: %zu bytes for p->imgs", __func__, p->numin*sizeof *p->imgs); /* Fill in the WCS information of each image. */ input_counter=p->numin; while(p->inputs) { /* Pop from the list of input images and get the info. */ status=0; img=&p->imgs[--input_counter]; img->name=gal_list_str_pop(&p->inputs); tmpfits=gal_fits_hdu_open_format(img->name, p->cp.hdu, 0); gal_fits_img_info(tmpfits, &p->type, &img->ndim, &img->dsize, NULL, NULL); img->wcs=gal_wcs_read_fitsptr(tmpfits, p->hstartwcs, p->hendwcs, &img->nwcs); if(img->wcs) { gal_wcs_decompose_pc_cdelt(img->wcs); status=wcshdo(0, img->wcs, &img->nwcskeys, &img->wcstxt); if(status) error(EXIT_FAILURE, 0, "wcshdo ERROR %d: %s", status, wcs_errmsg[status]); } else if(p->mode==IMGCROP_MODE_WCS) error(EXIT_FAILURE, 0, "the WCS structure of %s (hdu: %s) " "image is not recognized. So WCS mode cannot be used " "as input coordinates. You can try with pixel coordinates " "with `--mode=img'", img->name, p->cp.hdu); fits_close_file(tmpfits, &status); gal_fits_io_error(status, NULL); /* Make sure all the images have the same type and dimensions. */ if(firsttype==0) { /* Set the basic information. */ firsttype = p->type; firstndim = img->ndim; p->bitnul = gal_fits_key_img_blank(p->type); /* Make sure the number of dimensions is supported. */ if(firstndim>MAXDIM) error(EXIT_FAILURE, 0, "%s: is as %zu dimensional dataset, Crop " "currently only supports a maximum of %d dimensions", img->name, firstndim, MAXDIM); /* Make sure the number of coordinates given for center correspond to the dimensionality of the data. */ if(p->center && p->center->size!=firstndim) error(EXIT_FAILURE, 0, "%s (hdu %s) has %zu dimensions, but " "%zu coordinates were given to `--center'", img->name, p->cp.hdu, firstndim, p->center->size); } else { if(firsttype!=p->type) error(EXIT_FAILURE, 0, "%s: type is `%s' while previous input(s) " "were `%s' type. All inputs must have the same pixel data " "type.\n\nYou can use Gnuastro's Arithmetic program to " "convert `%s' to `%s', please run this command for more " "information (press `SPACE' for going down and `q' to " "return to the command-line):\n\n" " $ info Arithmetic\n", img->name, gal_type_name(p->type, 1), gal_type_name(firsttype, 1), img->name, gal_type_name(p->type, 1)); if(firstndim!=img->ndim) error(EXIT_FAILURE, 0, "%s: type has %zu dimensions, while " "previous input(s) had %zu dimensions. All inputs must " "have the same number of dimensions", img->name, img->ndim, firstndim); } /* In WCS mode, we need some additional preparations. */ if(p->mode==IMGCROP_MODE_WCS) wcsmode_check_prepare(p, img); } /* Unify central crop methods into `p->centercoords'. */ if(p->catname || p->center) ui_prepare_center(p); /* `ui_read_cols' set the number of output crops when a catalog was given, in all other cases, we only have one output. */ if(p->catname==NULL) p->numout=1; /* Prepare the log file if the user has asked for it. */ ui_make_log(p); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct cropparams *p) { char *msg; struct timeval t1; struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* To see how long it takes to read meta-data. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Report timing: */ if(!p->cp.quiet) { printf(PROGRAM_NAME" started on %s", ctime(&p->rawtime)); asprintf(&msg, "Read metadata of %zu dataset%s.", p->numin, p->numin>1 ? "s" : ""); gal_timing_report(&t1, msg, 1); if(p->numout>1) { asprintf(&msg, "Will try making %zu crops (from catalog).", p->numout); gal_timing_report(NULL, msg, 1); } } } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct cropparams *p, struct timeval *t1) { size_t i; /* Free the simple arrays (if they were set). */ gal_data_free(p->center); if(p->cp.hdu) free(p->cp.hdu); if(p->cathdu) free(p->cathdu); if(p->catname) free(p->catname); /* The arguments (note that the values were not allocated). */ gal_list_str_free(p->inputs, 0); /* Free the name/ array. */ if(p->name) { for(i=0;i<p->numout;++i) free(p->name[i]); free(p->name); } /* Free the log information. */ if(p->cp.log) gal_list_data_free(p->log); /* Print the final message. */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); } ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/main.c������������������������������������������������������������������������0000644�0001750�0001750�00000003051�13121462410�012735� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Crop - Crop a given size from one or multiple images. Crop is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "crop.h" #include "onecrop.h" int main (int argc, char *argv[]) { struct timeval t1; struct cropparams p={{{0},0},0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run Image Crop */ crop(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully.*/ return EXIT_SUCCESS; } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/Makefile.in�������������������������������������������������������������������0000644�0001750�0001750�00000211556�13217217705�013740� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright (C) 1994-2017 Free Software Foundation, Inc. # This Makefile.in is free software; the Free Software Foundation # gives unlimited permission to copy and/or distribute it, # with or without modifications, as long as this notice is preserved. # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY, to the extent permitted by law; without # even the implied warranty of MERCHANTABILITY or FITNESS FOR A # PARTICULAR PURPOSE. @SET_MAKE@ VPATH = @srcdir@ am__is_gnu_make = { \ if test -z '$(MAKELEVEL)'; then \ false; \ elif test -n '$(MAKE_HOST)'; then \ true; \ elif test -n '$(MAKE_VERSION)' && test -n '$(CURDIR)'; then \ true; \ else \ false; \ fi; \ } am__make_running_with_option = \ case $${target_option-} in \ ?) ;; \ *) echo "am__make_running_with_option: internal error: invalid" \ "target option '$${target_option-}' specified" >&2; \ exit 1;; \ esac; \ has_opt=no; \ 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GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Crop. # Crop is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astcrop --help # Full list of options, short doc. # $ astcrop -P # Print all options and used values. # $ info astcrop # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Input image and catalog parameters: cathdu 1 hstartwcs 0 hendwcs 0 # Output parameters: checkcenter 0 suffix _cropped.fits # Crop by center (when a catalog is given) coordcol 2 coordcol 3 # Operating mode: mode wcs ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/crop/Makefile.am�������������������������������������������������������������������0000644�0001750�0001750�00000002622�13121462410�013704� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astcrop astcrop_LDADD = -lgnuastro astcrop_SOURCES = main.c ui.c crop.c wcsmode.c onecrop.c EXTRA_DIST = main.h authors-cite.h args.h ui.h crop.h wcsmode.h onecrop.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.ma dist_sysconf_DATA = astcrop.conf ��������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/�������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�012731� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/cosmiccal.h��������������������������������������������������������������0000644�0001750�0001750�00000002252�13174362166�014766� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef COSMICCAL_H #define COSMICCAL_H /* Format of final outputs */ # define FLTFORMAT " - %-55s%f\n" # define EXPFORMAT " - %-55s%e\n" void cosmiccal(struct cosmiccalparams *p); #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/ui.h���������������������������������������������������������������������0000644�0001750�0001750�00000004271�13174462540�013446� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_SPECIFIC = GAL_OPTIONS_GROUP_AFTER_COMMON, }; /* Available letters for short options: e f i j k n p t w x y B E J O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_REDSHIFT = 'z', UI_KEY_H0 = 'H', UI_KEY_OLAMBDA = 'l', UI_KEY_OMATTER = 'm', UI_KEY_ORADIATION = 'r', UI_KEY_AGENOW = 'G', UI_KEY_CRITICALDENSITYNOW = 'C', UI_KEY_PROPERDISTANCE = 'd', UI_KEY_ANGULARDIMDIST = 'A', UI_KEY_ARCSECTANDIST = 's', UI_KEY_LUMINOSITYDIST = 'L', UI_KEY_DISTANCEMODULUS = 'u', UI_KEY_ABSMAGCONV = 'a', UI_KEY_AGE = 'g', UI_KEY_LOOKBACKTIME = 'b', UI_KEY_CRITICALDENSITY = 'c', UI_KEY_VOLUME = 'v', /* Only with long version (start with a value 1000, the rest will be set automatically). */ }; void ui_read_check_inputs_setup(int argc, char *argv[], struct cosmiccalparams *p); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/args.h�������������������������������������������������������������������0000644�0001750�0001750�00000015567�13175442274�014002� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { { "redshift", UI_KEY_REDSHIFT, "FLT", 0, "Redshift of interest.", GAL_OPTIONS_GROUP_INPUT, &p->redshift, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "H0", UI_KEY_H0, "FLT", 0, "Current expansion rate (Hubble constant).", GAL_OPTIONS_GROUP_INPUT, &p->H0, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "olambda", UI_KEY_OLAMBDA, "FLT", 0, "Current cosmological cst. dens. per crit. dens.", GAL_OPTIONS_GROUP_INPUT, &p->olambda, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "omatter", UI_KEY_OMATTER, "FLT", 0, "Current matter density per critical density.", GAL_OPTIONS_GROUP_INPUT, &p->omatter, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "oradiation", UI_KEY_ORADIATION, "FLT", 0, "Current radiation density per critical density.", GAL_OPTIONS_GROUP_INPUT, &p->oradiation, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Specific calculations", UI_GROUP_SPECIFIC }, { "agenow", UI_KEY_AGENOW, 0, 0, "Age of universe now (Gyr).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "criticaldensitynow", UI_KEY_CRITICALDENSITYNOW, 0, 0, "Critical density now (g/cm^3).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "properdistance", UI_KEY_PROPERDISTANCE, 0, 0, "Proper distance to z (Mpc).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "angulardimdist", UI_KEY_ANGULARDIMDIST, 0, 0, "Angular diameter distance (Mpc).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "arcsectandist", UI_KEY_ARCSECTANDIST, 0, 0, "Tangential dist. covered by 1arcsec at z (kpc).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "luminositydist", UI_KEY_LUMINOSITYDIST, 0, 0, "Luminosity distance to z (Mpc).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "distancemodulus", UI_KEY_DISTANCEMODULUS, 0, 0, "Distance modulus at z (no units).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "absmagconv", UI_KEY_ABSMAGCONV, 0, 0, "Conversion to absolute magnitude (no unit).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "age", UI_KEY_AGE, 0, 0, "Age of universe at z (Gyr).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "lookbacktime", UI_KEY_LOOKBACKTIME, 0, 0, "Look back time to z (Gyr).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "criticaldensity", UI_KEY_CRITICALDENSITY, 0, 0, "Critical density at z (g/cm^3).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, { "volume", UI_KEY_VOLUME, 0, 0, "Comoving volume (4pi str) to z (Mpc^3).", UI_GROUP_SPECIFIC, &p->specific, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET, ui_add_to_single_value, }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif �����������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/authors-cite.h�����������������������������������������������������������0000644�0001750�0001750�00000003002�13211076737�015430� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/main.h�������������������������������������������������������������������0000644�0001750�0001750�00000004164�13174462540�013756� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro/list.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "CosmicCalculator" /* Program full name. */ #define PROGRAM_EXEC "astcosmiccal" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Main program parameters structure */ struct cosmiccalparams { /* Other structures: */ struct gal_options_common_params cp; /* Common parameters. */ /* Input: */ double redshift; /* Redshift of interest. */ double H0; /* Current expansion rate (km/sec/Mpc). */ double olambda; /* Current cosmological constant dens. */ double omatter; /* Current matter density. */ double oradiation; /* Current radiation density. */ /* Outputs. */ gal_list_i32_t *specific; /* Codes for single row calculations. */ /* Internal: */ time_t rawtime; /* Starting time of the program. */ }; #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/cosmiccal.c��������������������������������������������������������������0000644�0001750�0001750�00000023300�13174462540�014753� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <gnuastro/cosmology.h> #include "main.h" #include "ui.h" #include "cosmiccal.h" /**************************************************************/ /************ Main function *************/ /**************************************************************/ static void cosmiccal_print_input(struct cosmiccalparams *p) { printf("%s\n", PROGRAM_STRING); printf("\n Input parameters\n"); printf( " ----------------\n"); if( !isnan(p->redshift) ) printf(FLTFORMAT, "Desired redshift for calculations (z):", p->redshift); printf(FLTFORMAT, "Expansion rate (Hubble constant, H0), now:", p->H0); printf(FLTFORMAT, "Cosmological constant fractional density, now:", p->olambda); printf(FLTFORMAT, "Matter fractional density, now:", p->omatter); printf(EXPFORMAT, "Radiation fractional density, now:", p->oradiation); printf(EXPFORMAT, "Curvatue fractional density (from the above):", 1 - ( p->olambda + p->omatter + p->oradiation )); } static void cosmiccal_printall(struct cosmiccalparams *p) { double ad, ld, vz, pd, absmagconv; double curage, ccritd, distmod, outage, zcritd; /* The user wants everything, do all the calculations and print everything with full descriptions. */ curage=gal_cosmology_age(0.0f, p->H0, p->olambda, p->omatter, p->oradiation); ccritd=gal_cosmology_critical_density(0.0f, p->H0, p->olambda, p->omatter, p->oradiation); pd=gal_cosmology_proper_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); ad=gal_cosmology_angular_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); ld=gal_cosmology_luminosity_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); distmod=gal_cosmology_distance_modulus(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); absmagconv=gal_cosmology_to_absolute_mag(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); outage=gal_cosmology_age(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); zcritd=gal_cosmology_critical_density(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); vz=gal_cosmology_comoving_volume(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); /* Print out results: */ cosmiccal_print_input(p); printf("\n\n Universe now\n"); printf( " ------------\n"); printf(FLTFORMAT, "Age of Universe now (Gyr):", curage); printf(EXPFORMAT, "Critical density now (g/cm^3):", ccritd); printf(FLTFORMAT, "Proper distance to z (Mpc):", pd); printf(FLTFORMAT, "Angular diameter distance to z (Mpc):", ad); printf(FLTFORMAT, "Tangential distance covered by 1 arcsec at z (Kpc):", ad*1000*M_PI/3600/180); printf(FLTFORMAT, "Luminosity distance to z (Mpc):", ld); printf(FLTFORMAT, "Distance modulus at z (no unit):", distmod); printf(FLTFORMAT, "Conversion to absolute magnitude (no unit):", absmagconv); printf("\n\n Universe at desired redshift z\n"); printf( " ------------------------------\n"); printf(FLTFORMAT, "Age of Universe at z (Gyr):", outage); printf(FLTFORMAT, "Look-back time to z (Gyr):", curage-outage); printf(EXPFORMAT, "Critical density at z (g/cm^3):", zcritd); printf("\n\n Comoving universe (time independent)\n"); printf( " ------------------------------------\n"); printf(FLTFORMAT, "Comoving volume over 4pi stradian to z (Mpc^3):", vz); } void cosmiccal(struct cosmiccalparams *p) { gal_list_i32_t *tmp; double curage, zage; /* If no redshift is given, just print the input parameters along with a notice that further calculations are only possible with a redshift and abort. */ if(isnan(p->redshift)) { cosmiccal_print_input(p); printf("\n\nPlease specify a redshift with the `--redshift' (or `-z') " "option.\n"); return; } /* In case the user just wants one number, only print that and return. */ if(p->specific) { for(tmp=p->specific;tmp!=NULL;tmp=tmp->next) switch(tmp->v) { case UI_KEY_AGENOW: printf("%f ", gal_cosmology_age(0.0f, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_CRITICALDENSITYNOW: printf("%e ", gal_cosmology_critical_density(0.0f, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_PROPERDISTANCE: printf("%f ", gal_cosmology_proper_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_ANGULARDIMDIST: printf("%f ", gal_cosmology_angular_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_ARCSECTANDIST: printf("%f ", ( gal_cosmology_angular_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation) * 1000 * M_PI / 3600 / 180 ) ); break; case UI_KEY_LUMINOSITYDIST: printf("%f ", gal_cosmology_luminosity_distance(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_DISTANCEMODULUS: printf("%f ", gal_cosmology_distance_modulus(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_ABSMAGCONV: printf("%f ", gal_cosmology_to_absolute_mag(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_AGE: printf("%f ", gal_cosmology_age(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_LOOKBACKTIME: curage=gal_cosmology_age(0.0f, p->H0, p->olambda, p->omatter, p->oradiation); zage=gal_cosmology_age(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation); printf("%f ", curage-zage); break; case UI_KEY_CRITICALDENSITY: printf("%e ", gal_cosmology_critical_density(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; case UI_KEY_VOLUME: printf("%f ", gal_cosmology_comoving_volume(p->redshift, p->H0, p->olambda, p->omatter, p->oradiation)); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " "fix the problem. The code %d is not recognized as a " "single value calculation code", __func__, PACKAGE_BUGREPORT, tmp->v); } /* Print a new-line character to finish the output. */ printf("\n"); } else cosmiccal_printall(p); } ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/ui.c���������������������������������������������������������������������0000644�0001750�0001750�00000023640�13211076737�013443� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <gsl/gsl_const_mksa.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = ""; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will do cosmological " "calculations. If no redshfit is specified, it will only print the main " "input parameters. If only a redshift is given, it will print a table of " "all calculations. If any of the single row calculations are requested, " "only their values will be printed with a single space between each.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct cosmiccalparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* Program specific initializations. */ p->redshift = NAN; /* Modify the common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_OUTPUT: case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } /* Select specific options. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_QUIET: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_NUMTHREADS: case GAL_OPTIONS_KEY_MINMAPSIZE: case GAL_OPTIONS_KEY_IGNORECASE: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct cosmiccalparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: argp_error(state, "currently %s doesn't take any arguments", PROGRAM_NAME); break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } static void * ui_add_to_single_value(struct argp_option *option, char *arg, char *filename, size_t lineno, void *params) { /* In case of printing the option values. */ if(lineno==-1) error(EXIT_FAILURE, 0, "currently the options to be printed in one row " "(like `--age', `--luminositydist', and etc) do not support " "printing with the `--printparams' (`-P'), or writing into " "configuration files due to lack of time when implementing " "these features. You can put them into configuration files " "manually. Please get in touch with us at `%s', so we can " "implement it", PACKAGE_BUGREPORT); /* If this option is given in a configuration file, then `arg' will not be NULL and we don't want to do anything if it is `0'. */ if(arg) { /* Make sure the value is only `0' or `1'. */ if( arg[1]!='\0' && *arg!='0' && *arg!='1' ) error_at_line(EXIT_FAILURE, 0, filename, lineno, "the `--%s' " "option takes no arguments. In a configuration " "file it can only have the values `1' or `0', " "indicating if it should be used or not", option->name); /* Only proceed if the (possibly given) argument is 1. */ if(arg[0]=='0' && arg[1]=='\0') return NULL; } /* Add this option to the print list and return. */ gal_list_i32_add(option->value, option->key); return NULL; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct cosmiccalparams *p) { double sum = p->olambda + p->omatter + p->oradiation; /* Check if the density fractions add up to 1 (within floating point error). */ if( sum > (1+1e-8) || sum < (1-1e-8) ) error(EXIT_FAILURE, 0, "sum of fractional densities is not 1, but %.8f. " "The cosmological constant (`olambda'), matter (`omatter') " "and radiation (`oradiation') densities are given as %.8f, %.8f, " "%.8f", sum, p->olambda, p->omatter, p->oradiation); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ static void ui_preparations(struct cosmiccalparams *p) { /* The list is filled out in a first-in-last-out order. By the time control reaches here, the list is finalized. So we should just reverse it so the user gets values in the same order they requested them. */ gal_list_i32_reverse(&p->specific); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct cosmiccalparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } ������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/main.c�������������������������������������������������������������������0000644�0001750�0001750�00000003040�13174364642�013745� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* CosmicCalculator - Calculate cosmological parameters CosmicCalculator is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" /* needs main.h. */ #include "cosmiccal.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct cosmiccalparams p={{{0},0},0}; /* Get the starting time. */ time(&p.rawtime); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ cosmiccal(&p); /* Return successfully.*/ return EXIT_SUCCESS; } 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@GNULIB_ATAN2F@ GNULIB_ATANF = @GNULIB_ATANF@ GNULIB_ATANL = @GNULIB_ATANL@ GNULIB_ATOLL = @GNULIB_ATOLL@ GNULIB_BIND = @GNULIB_BIND@ GNULIB_BTOWC = @GNULIB_BTOWC@ GNULIB_CALLOC_POSIX = @GNULIB_CALLOC_POSIX@ GNULIB_CANONICALIZE_FILE_NAME = @GNULIB_CANONICALIZE_FILE_NAME@ GNULIB_CBRT = @GNULIB_CBRT@ GNULIB_CBRTF = @GNULIB_CBRTF@ GNULIB_CBRTL = @GNULIB_CBRTL@ GNULIB_CEIL = @GNULIB_CEIL@ GNULIB_CEILF = @GNULIB_CEILF@ GNULIB_CEILL = @GNULIB_CEILL@ GNULIB_CHDIR = @GNULIB_CHDIR@ GNULIB_CHOWN = @GNULIB_CHOWN@ GNULIB_CLOSE = @GNULIB_CLOSE@ GNULIB_CONNECT = @GNULIB_CONNECT@ GNULIB_COPYSIGN = @GNULIB_COPYSIGN@ GNULIB_COPYSIGNF = @GNULIB_COPYSIGNF@ GNULIB_COPYSIGNL = @GNULIB_COPYSIGNL@ GNULIB_COSF = @GNULIB_COSF@ GNULIB_COSHF = @GNULIB_COSHF@ GNULIB_COSL = @GNULIB_COSL@ GNULIB_CTIME = @GNULIB_CTIME@ GNULIB_DPRINTF = @GNULIB_DPRINTF@ GNULIB_DUP = @GNULIB_DUP@ GNULIB_DUP2 = @GNULIB_DUP2@ GNULIB_DUP3 = @GNULIB_DUP3@ GNULIB_DUPLOCALE = @GNULIB_DUPLOCALE@ GNULIB_ENVIRON = @GNULIB_ENVIRON@ GNULIB_EUIDACCESS = @GNULIB_EUIDACCESS@ GNULIB_EXP2 = @GNULIB_EXP2@ GNULIB_EXP2F = @GNULIB_EXP2F@ GNULIB_EXP2L = @GNULIB_EXP2L@ GNULIB_EXPF = @GNULIB_EXPF@ GNULIB_EXPL = @GNULIB_EXPL@ GNULIB_EXPLICIT_BZERO = @GNULIB_EXPLICIT_BZERO@ GNULIB_EXPM1 = @GNULIB_EXPM1@ GNULIB_EXPM1F = @GNULIB_EXPM1F@ GNULIB_EXPM1L = @GNULIB_EXPM1L@ GNULIB_FABSF = @GNULIB_FABSF@ GNULIB_FABSL = @GNULIB_FABSL@ GNULIB_FACCESSAT = @GNULIB_FACCESSAT@ GNULIB_FCHDIR = @GNULIB_FCHDIR@ GNULIB_FCHMODAT = @GNULIB_FCHMODAT@ GNULIB_FCHOWNAT = @GNULIB_FCHOWNAT@ GNULIB_FCLOSE = @GNULIB_FCLOSE@ GNULIB_FCNTL = @GNULIB_FCNTL@ GNULIB_FDATASYNC = @GNULIB_FDATASYNC@ GNULIB_FDOPEN = @GNULIB_FDOPEN@ GNULIB_FFLUSH = @GNULIB_FFLUSH@ GNULIB_FFS = @GNULIB_FFS@ GNULIB_FFSL = @GNULIB_FFSL@ GNULIB_FFSLL = @GNULIB_FFSLL@ GNULIB_FGETC = @GNULIB_FGETC@ GNULIB_FGETS = @GNULIB_FGETS@ GNULIB_FLOOR = @GNULIB_FLOOR@ GNULIB_FLOORF = @GNULIB_FLOORF@ GNULIB_FLOORL = @GNULIB_FLOORL@ GNULIB_FMA = @GNULIB_FMA@ GNULIB_FMAF = @GNULIB_FMAF@ GNULIB_FMAL = @GNULIB_FMAL@ GNULIB_FMOD = @GNULIB_FMOD@ GNULIB_FMODF = @GNULIB_FMODF@ GNULIB_FMODL = @GNULIB_FMODL@ GNULIB_FOPEN = @GNULIB_FOPEN@ GNULIB_FPRINTF = @GNULIB_FPRINTF@ GNULIB_FPRINTF_POSIX = @GNULIB_FPRINTF_POSIX@ GNULIB_FPURGE = @GNULIB_FPURGE@ GNULIB_FPUTC = @GNULIB_FPUTC@ GNULIB_FPUTS = @GNULIB_FPUTS@ GNULIB_FREAD = @GNULIB_FREAD@ GNULIB_FREOPEN = @GNULIB_FREOPEN@ GNULIB_FREXP = @GNULIB_FREXP@ GNULIB_FREXPF = @GNULIB_FREXPF@ GNULIB_FREXPL = @GNULIB_FREXPL@ GNULIB_FSCANF = @GNULIB_FSCANF@ GNULIB_FSEEK = @GNULIB_FSEEK@ GNULIB_FSEEKO = @GNULIB_FSEEKO@ GNULIB_FSTAT = @GNULIB_FSTAT@ GNULIB_FSTATAT = @GNULIB_FSTATAT@ GNULIB_FSYNC = @GNULIB_FSYNC@ GNULIB_FTELL = @GNULIB_FTELL@ GNULIB_FTELLO = @GNULIB_FTELLO@ GNULIB_FTRUNCATE = @GNULIB_FTRUNCATE@ GNULIB_FUTIMENS = @GNULIB_FUTIMENS@ GNULIB_FWRITE = @GNULIB_FWRITE@ GNULIB_GETC = @GNULIB_GETC@ GNULIB_GETCHAR = @GNULIB_GETCHAR@ GNULIB_GETCWD = @GNULIB_GETCWD@ GNULIB_GETDELIM = @GNULIB_GETDELIM@ GNULIB_GETDOMAINNAME = @GNULIB_GETDOMAINNAME@ GNULIB_GETDTABLESIZE = @GNULIB_GETDTABLESIZE@ GNULIB_GETGROUPS = @GNULIB_GETGROUPS@ GNULIB_GETHOSTNAME = @GNULIB_GETHOSTNAME@ GNULIB_GETLINE = @GNULIB_GETLINE@ GNULIB_GETLOADAVG = @GNULIB_GETLOADAVG@ GNULIB_GETLOGIN = @GNULIB_GETLOGIN@ GNULIB_GETLOGIN_R = @GNULIB_GETLOGIN_R@ GNULIB_GETPAGESIZE = @GNULIB_GETPAGESIZE@ GNULIB_GETPEERNAME = @GNULIB_GETPEERNAME@ GNULIB_GETSOCKNAME = @GNULIB_GETSOCKNAME@ GNULIB_GETSOCKOPT = @GNULIB_GETSOCKOPT@ GNULIB_GETSUBOPT = @GNULIB_GETSUBOPT@ GNULIB_GETTIMEOFDAY = @GNULIB_GETTIMEOFDAY@ GNULIB_GETUSERSHELL = @GNULIB_GETUSERSHELL@ GNULIB_GL_UNISTD_H_GETOPT = @GNULIB_GL_UNISTD_H_GETOPT@ GNULIB_GRANTPT = @GNULIB_GRANTPT@ GNULIB_GROUP_MEMBER = @GNULIB_GROUP_MEMBER@ GNULIB_HYPOT = @GNULIB_HYPOT@ GNULIB_HYPOTF = @GNULIB_HYPOTF@ GNULIB_HYPOTL = @GNULIB_HYPOTL@ GNULIB_ILOGB = @GNULIB_ILOGB@ GNULIB_ILOGBF = @GNULIB_ILOGBF@ GNULIB_ILOGBL = @GNULIB_ILOGBL@ GNULIB_IMAXABS = @GNULIB_IMAXABS@ GNULIB_IMAXDIV = @GNULIB_IMAXDIV@ GNULIB_INET_NTOP = @GNULIB_INET_NTOP@ GNULIB_INET_PTON = @GNULIB_INET_PTON@ GNULIB_IOCTL = @GNULIB_IOCTL@ GNULIB_ISATTY = @GNULIB_ISATTY@ GNULIB_ISBLANK = @GNULIB_ISBLANK@ GNULIB_ISFINITE = @GNULIB_ISFINITE@ GNULIB_ISINF = @GNULIB_ISINF@ GNULIB_ISNAN = @GNULIB_ISNAN@ GNULIB_ISNAND = @GNULIB_ISNAND@ GNULIB_ISNANF = @GNULIB_ISNANF@ GNULIB_ISNANL = @GNULIB_ISNANL@ GNULIB_ISWBLANK = @GNULIB_ISWBLANK@ GNULIB_ISWCTYPE = @GNULIB_ISWCTYPE@ GNULIB_LCHMOD = @GNULIB_LCHMOD@ GNULIB_LCHOWN = @GNULIB_LCHOWN@ GNULIB_LDEXPF = @GNULIB_LDEXPF@ GNULIB_LDEXPL = @GNULIB_LDEXPL@ GNULIB_LINK = @GNULIB_LINK@ GNULIB_LINKAT = @GNULIB_LINKAT@ GNULIB_LISTEN = @GNULIB_LISTEN@ GNULIB_LOCALECONV = @GNULIB_LOCALECONV@ GNULIB_LOCALTIME = @GNULIB_LOCALTIME@ GNULIB_LOG = @GNULIB_LOG@ GNULIB_LOG10 = @GNULIB_LOG10@ GNULIB_LOG10F = @GNULIB_LOG10F@ GNULIB_LOG10L = @GNULIB_LOG10L@ GNULIB_LOG1P = @GNULIB_LOG1P@ GNULIB_LOG1PF = @GNULIB_LOG1PF@ GNULIB_LOG1PL = @GNULIB_LOG1PL@ GNULIB_LOG2 = @GNULIB_LOG2@ GNULIB_LOG2F = @GNULIB_LOG2F@ GNULIB_LOG2L = @GNULIB_LOG2L@ GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ 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pdf-am ps ps-am tags tags-am uninstall \ uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/astcosmiccal.conf��������������������������������������������������������0000644�0001750�0001750�00000002661�13174462540�016175� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for CosmicCalculator. # CosmicCalculator is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astcosmiccal --help # Full list of options, short doc. # $ astcosmiccal -P # Print all options and used values. # $ info astcosmiccal # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Citation # ======== # # The current default cosmological values in CosmicCalculator are taken # from the Planck 2015 results (paper XIII, A&A 594, A13 (2016), Table 4, # page 31, last column: "TT,TE,EE+lowP+lensing+ext"). # # http://www.aanda.org/articles/aa/full_html/2016/10/aa25830-15/aa25830-15.html # # IMPORTANT NOTES: If you change these system-wide default values, please # change this comment and cite the source. # Input: H0 67.74 olambda 0.6911 omatter 0.3089 oradiation 0.0 # Output: �������������������������������������������������������������������������������gnuastro-0.5/bin/cosmiccal/Makefile.am��������������������������������������������������������������0000644�0001750�0001750�00000002610�13121462410�014673� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2016, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astcosmiccal astcosmiccal_LDADD = -lgnuastro astcosmiccal_SOURCES = main.c ui.c cosmiccal.c EXTRA_DIST = main.h authors-cite.h args.h ui.h cosmiccal.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astcosmiccal.conf ������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/��������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�012627� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/convolve.h����������������������������������������������������������������0000644�0001750�0001750�00000003522�13121462410�014544� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef CONVOLVE_H #define CONVOLVE_H #include <gnuastro/threads.h> #include <gsl/gsl_fft_complex.h> struct fftonthreadparams { /* Operating info: */ size_t id; /* The number of this thread. */ struct convolveparams *p; /* Pointer to main program structure. */ int forward1backwardn1; /* Operate on one or two images. */ size_t stride; /* 1D FFT on rows or columns? */ /* Pointers to GSL FFT structures: */ gsl_fft_complex_wavetable *ps0wave; gsl_fft_complex_wavetable *ps1wave; gsl_fft_complex_workspace *ps0work; gsl_fft_complex_workspace *ps1work; /* Thread parameters. */ size_t *indexs; /* Indexs to be used in this thread. */ pthread_barrier_t *b; /* Barrier to keep threads waiting. */ }; void convolve(struct convolveparams *p); #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/ui.h����������������������������������������������������������������������0000644�0001750�0001750�00000003753�13174462540�013350� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program. */ enum program_args_groups { UI_GROUP_MESH_GRID = GAL_OPTIONS_GROUP_AFTER_COMMON, }; /* Available letters for short options: a b e f g i j l n p s v w x y z A B E G J L O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_KERNEL = 'k', UI_KEY_KHDU = 'u', UI_KEY_MINSHARPSPEC = 'H', UI_KEY_CHECKFREQSTEPS = 'C', UI_KEY_TILESIZE = 't', UI_KEY_NUMCHANNELS = 'c', UI_KEY_REMAINDERFRAC = 'r', UI_KEY_DOMAIN = 'd', UI_KEY_MAKEKERNEL = 'm', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_NOKERNELFLIP = 1000, UI_KEY_NOKERNELNORM, UI_KEY_NOEDGECORRECTION, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct convolveparams *p); void ui_free_report(struct convolveparams *p, struct timeval *t1); #endif ���������������������gnuastro-0.5/bin/convolve/args.h��������������������������������������������������������������������0000644�0001750�0001750�00000010471�13121462410�013646� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { /* Inputs */ { "kernel", UI_KEY_KERNEL, "STR", 0, "File name of kernel for convolution.", GAL_OPTIONS_GROUP_INPUT, &p->kernelname, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "khdu", UI_KEY_KHDU, "STR", 0, "HDU containing the kernel.", GAL_OPTIONS_GROUP_INPUT, &p->khdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "nokernelflip", UI_KEY_NOKERNELFLIP, 0, 0, "Do not flip the kernel image.", GAL_OPTIONS_GROUP_INPUT, &p->nokernelflip, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "nokernelnorm", UI_KEY_NOKERNELNORM, 0, 0, "Do not normalize the kernel image.", GAL_OPTIONS_GROUP_INPUT, &p->nokernelnorm, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "minsharpspec", UI_KEY_MINSHARPSPEC, "FLT", 0, "Deconvolution: min spectrum of sharp img.", GAL_OPTIONS_GROUP_INPUT, &p->minsharpspec, GAL_TYPE_FLOAT64, GAL_OPTIONS_RANGE_GE_0_LE_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Outputs */ { "checkfreqsteps", UI_KEY_CHECKFREQSTEPS, 0, 0, "View the steps in the frequency domain.", GAL_OPTIONS_GROUP_OUTPUT, &p->checkfreqsteps, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "noedgecorrection", UI_KEY_NOEDGECORRECTION, 0, 0, "Do not correct the edges in the spatial domain", GAL_OPTIONS_GROUP_OUTPUT, &p->noedgecorrection, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, /* Operating mode. */ { "domain", UI_KEY_DOMAIN, "STR", 0, "Convolution domain: `spatial', `frequency'.", GAL_OPTIONS_GROUP_OPERATING_MODE, &p->domainstr, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_MANDATORY, GAL_OPTIONS_NOT_SET }, { "makekernel", UI_KEY_MAKEKERNEL, "INT", 0, "Make 2*INT kernel to create input image.", GAL_OPTIONS_GROUP_OPERATING_MODE, &p->makekernel, GAL_TYPE_SIZE_T, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/authors-cite.h������������������������������������������������������������0000644�0001750�0001750�00000002771�13211076737�015342� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif �������gnuastro-0.5/bin/convolve/main.h��������������������������������������������������������������������0000644�0001750�0001750�00000006632�13121462410�013642� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Program names. */ #define PROGRAM_NAME "Convolve" /* Program full name. */ #define PROGRAM_EXEC "astconvolve" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Macros */ #define CONVFLOATINGPOINTERR 1e-10 /* Enumerators */ enum complex_to_real { COMPLEX_TO_REAL_INVALID, /* ==0 by C standard. */ COMPLEX_TO_REAL_SPEC, COMPLEX_TO_REAL_PHASE, COMPLEX_TO_REAL_REAL, }; enum domain_codes { CONVOLVE_DOMAIN_INVALID, /* ==0 by C standard. */ CONVOLVE_DOMAIN_SPATIAL, CONVOLVE_DOMAIN_FREQUENCY, }; /* Processing parameters structure */ struct convolveparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ char *filename; /* Name of input file. */ char *kernelname; /* File name of kernel. */ char *khdu; /* HDU of kernel. */ uint8_t nokernelflip; /* Do not flip the kernel. */ uint8_t nokernelnorm; /* Do not normalize the kernel. */ double minsharpspec; /* Deconvolution: min spect. of sharp img. */ uint8_t checkfreqsteps; /* View the frequency domain steps. */ char *domainstr; /* String value specifying domain. */ size_t makekernel; /* Make a kernel to create input. */ uint8_t noedgecorrection; /* Do not correct spatial edge effects. */ /* Internal */ int domain; /* Frequency or spatial domain conv. */ gal_data_t *input; /* Input image array. */ gal_data_t *kernel; /* Input Kernel array. */ double *pimg; /* Padded image array. */ double *pker; /* Padded kernel array. */ double *rpad; /* Real final image before removing pad'd. */ size_t ps0; /* Padded size along first C axis. */ size_t ps1; /* Padded size along second C axis. */ char *freqstepsname; /* Name of file to check frequency steps. */ time_t rawtime; /* Starting time of the program. */ }; #endif ������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/convolve.c����������������������������������������������������������������0000644�0001750�0001750�00000056352�13151366335�014564� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <gsl/gsl_errno.h> #include <gnuastro/wcs.h> #include <gnuastro/tile.h> #include <gnuastro/fits.h> #include <gnuastro/threads.h> #include <gnuastro/convolve.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "convolve.h" /******************************************************************/ /************* Complex numbers *****************/ /******************************************************************/ /* We have a complex (R+iI) array and we want to display it. But we can only do that either with the spectrum, or the phase: Spectrum: sqrt(R^2+I^2) Phase: arctan(I/R) */ void complextoreal(double *c, size_t size, int action, double **output) { double *out, *o, *of; /* Allocate the space for the real array. */ *output=out=gal_data_malloc_array(GAL_TYPE_FLOAT64, size, __func__, "output"); /* Fill the real array with the derived value from the complex array. */ of=(o=out)+size; switch(action) { case COMPLEX_TO_REAL_SPEC: do { *o++ = sqrt( *c**c + *(c+1)**(c+1) ); c+=2; } while(o<of); break; case COMPLEX_TO_REAL_PHASE: do { *o++ = atan2( *(c+1), *c ); c+=2; } while(o<of); break; case COMPLEX_TO_REAL_REAL: do { *o++ = *c; c+=2; } while(o<of); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s so we can " "correct it. The `action' code %d is not recognized", __func__, PACKAGE_BUGREPORT, action); } } /* Multily two complex arrays and save the result in the first: (a+ib)*(c+id)=ac+iad+ibc-bd=(ac-bd)+i(ad-bc) The loop is easy to understand: we want to replace two variables. But changing one, will affect the other. So what we do, is to store the final value of one, then replace the second, then finally replace the first one. Here, we first get the real component but don't put it in the output. Then we find and replace the imaginary component, finally, we put the new real component in the image. */ void complexarraymultiply(double *a, double *b, size_t size) { double r, *af; af=a+2*size; do { r = (*a * *b) - (*(a+1) * *(b+1)); *(a+1) = (*(a+1) * *b) + (*a * *(b+1)); *a++=r; /* Go onto (set) the imaginary part of a. */ b+=2; } while(++a<af); /* Go onto the next complex number. */ } /* Divide the elements of the first array by the elements of the second array and put the result into the elements of the first array. (a+ib)/(c+id)=[(a+ib)*(c-id)]/[(c+id)*(c-id)] =(ac-iad+ibc+bd)/(c^2+d^2) =[(ac+bd)+i(bc-ad)]/(c^2+d^2) See the explanations above complexarraymultiply for an explanation on the loop. */ void complexarraydivide(double *a, double *b, size_t size, double minsharpspec) { double r, *af; af=a+2*size; do { if (sqrt(*b**b + *(b+1)**(b+1))>minsharpspec) { r = ( ( (*a * *b) + (*(a+1) * *(b+1)) ) / ( *b * *b + *(b+1) * *(b+1) ) ); *(a+1) = ( ( (*(a+1) * *b) - (*a * *(b+1)) ) / ( *b * *b + *(b+1) * *(b+1) ) ); *a=r; /* Just as a sanity check (the result should never be larger than one. */ if(sqrt(*a**a + *(a+1)**(a+1))>1.00001f) *a=*(a+1)=0.0f; } else { *a=0; *(a+1)=0; } a+=2; b+=2; } while(a<af); /* Go onto the next complex number. */ } /******************************************************************/ /************* Padding and initializing *****************/ /******************************************************************/ void frequency_make_padded_complex(struct convolveparams *p) { size_t i, ps0, ps1; double *o, *op, *pimg, *pker; size_t is0=p->input->dsize[0], is1=p->input->dsize[1]; size_t ks0=p->kernel->dsize[0], ks1=p->kernel->dsize[1]; float *f, *ff, *input=p->input->array, *kernel=p->kernel->array; /* Find the sizes of the padded image, note that since the kernel sizes are always odd, the extra padding on the input image is always going to be an even number (clearly divisable). */ ps0=p->ps0 = p->makekernel ? is0 : is0 + ks0 - 1; ps1=p->ps1 = p->makekernel ? is1 : is1 + ks1 - 1; /* The Discrete Fourier transforms operate faster on even-sized arrays. So if the padded sides are not even, make them so: */ if(ps0%2) ps0=p->ps0=ps0+1; if(ps1%2) ps1=p->ps1=ps1+1; /* Allocate the space for the padded input image and fill it. */ pimg=p->pimg=gal_data_malloc_array(GAL_TYPE_FLOAT64, 2*ps0*ps1, __func__, "pimg"); for(i=0;i<ps0;++i) { op=(o=pimg+i*2*ps1)+2*ps1; /* pimg is complex. */ if(i<is0) { ff=(f=input+i*is1)+is1; do {*o++=*f; *o++=0.0f;} while(++f<ff); } do *o++=0.0f; while(o<op); } /* Allocate the space for the padded Kernel and fill it. */ pker=p->pker=gal_data_malloc_array(GAL_TYPE_FLOAT64, 2*ps0*ps1, __func__, "pker"); for(i=0;i<ps0;++i) { op=(o=pker+i*2*ps1)+2*ps1; /* pker is complex. */ if(i<ks0) { ff=(f=kernel+i*ks1)+ks1; do {*o++=*f; *o++=0.0f;} while(++f<ff); } do *o++=0.0f; while(o<op); } } /* Remove the padding from the final convolved image and also correct for roundoff errors. NOTE: The padding to the input image (on the first axis for example) was `p->kernel->dsize[0]-1'. Since `p->kernel->dsize[0]' is always odd, the padding will always be even. */ void removepaddingcorrectroundoff(struct convolveparams *p) { size_t ps1=p->ps1; size_t *isize=p->input->dsize; float *o, *input=p->input->array; double *d, *df, *start, *rpad=p->rpad; size_t i, hi0, hi1, mkwidth=2*p->makekernel-1; /* Set all the necessary parameters to crop the desired region. hi0 and hi1 are the coordinates of the first pixel in the output image. In the case of deconvolution, if the maximum radius is larger than the input image, we will also only be using region that contains non-zero rows and columns.*/ if(p->makekernel) { hi0 = mkwidth < isize[0] ? p->ps0/2-p->makekernel : 0; hi1 = mkwidth < isize[1] ? p->ps1/2-p->makekernel : 0; isize[0] = mkwidth < isize[0] ? 2*p->makekernel-1 : isize[0]; isize[1] = mkwidth < isize[1] ? 2*p->makekernel-1 : isize[1]; } else { hi0 = ( p->kernel->dsize[0] - 1 )/2; hi1 = ( p->kernel->dsize[1] - 1 )/2; } /* To start with, `start' points to the first pixel in the final image: */ start=&rpad[hi0*ps1+hi1]; for(i=0;i<isize[0];++i) { o = &input[ i * isize[1] ]; df = ( d = start + i * ps1 ) + isize[1]; do *o++ = ( *d<-CONVFLOATINGPOINTERR || *d>CONVFLOATINGPOINTERR ) ? *d : 0.0f; while (++d<df); } } /* Allocate the necessary arrays, note that we put everything in the first element of the fftonthreadparams structure array. All the other elements will point to this one later. This structure will be given to threads to run two times with a fixed set of parameters, that is why we are doing this here to facilitate the job. */ void fftinitializer(struct convolveparams *p, struct fftonthreadparams **outfp) { size_t i; struct fftonthreadparams *fp; /* Allocate the fftonthreadparams array. */ errno=0; *outfp=fp=malloc(p->cp.numthreads*sizeof *fp); if(fp==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for fp", __func__, p->cp.numthreads*sizeof *fp); /* Initialize the gsl_fft_wavetable structures (these are thread safe): */ fp[0].ps0wave=gsl_fft_complex_wavetable_alloc(p->ps0); fp[0].ps1wave=gsl_fft_complex_wavetable_alloc(p->ps1); /* Set the values for all the other threads: */ for(i=0;i<p->cp.numthreads;++i) { fp[i].p=p; fp[i].ps0wave=fp[0].ps0wave; fp[i].ps1wave=fp[0].ps1wave; fp[i].ps0work=gsl_fft_complex_workspace_alloc(p->ps0); fp[i].ps1work=gsl_fft_complex_workspace_alloc(p->ps1); } } void freefp(struct fftonthreadparams *fp) { size_t i; gsl_fft_complex_wavetable_free(fp[0].ps0wave); gsl_fft_complex_wavetable_free(fp[0].ps1wave); for(i=0;i<fp->p->cp.numthreads;++i) { gsl_fft_complex_workspace_free(fp[i].ps0work); gsl_fft_complex_workspace_free(fp[i].ps1work); } free(fp); } /* Unfortunately I don't understand why the division operation in deconvolution (makekernel) does not produce a centered image, the image is translated by half the input size in both dimensions. So I am correcting this in the spatial domain here. */ void correctdeconvolve(struct convolveparams *p, double **spatial) { double r, *s, *n, *d, *df, sum=0.0f; size_t i, j, ps0=p->ps0, ps1=p->ps1; int ii, jj, ci=p->ps0/2-1, cj=p->ps1/2-1; /* Check if the image has even sides. */ if(ps0%2 || ps1%2) error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s. The padded " "image sides are not an even number", __func__, PACKAGE_BUGREPORT); /* First convert the complex image to a real image: */ complextoreal(p->pimg, ps0*ps1, COMPLEX_TO_REAL_SPEC, &s); /* Allocate the array to keep the new values */ errno=0; n=malloc(ps0*ps1*sizeof *n); if(n==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `n'", __func__, ps0*ps1*sizeof *n); /* Put the elements in their proper place: For example in one dimention where the values are actually the true distances: s[0]=0, s[1]=1, s[2]=2, s[3]=3, s[4]=4, s[5]=5 We want the value 0 to be in the `center'. Note that `s' is periodic, for example the next 6 elements have distances: s[6]=0, s[7]=1, s[8]=2, s[9]=3, s[10]=4, s[11]=5 So a `center'ed array would be like: s[0]=4, s[1]=5, s[2]=0, s[3]=1, s[4]=2, s[5]=3 The relations between the old (i and j) and new (ii and jj) come from something like the above line. */ for(i=0;i<ps0;++i) { ii= i>ps0/2 ? i-(ps0/2+1) : i+ps0/2-1; for(j=0;j<ps1;++j) { jj = j>ps1/2 ? j-(ps1/2+1) : j+ps1/2-1; r=sqrt( (ii-ci)*(ii-ci) + (jj-cj)*(jj-cj) ); sum += n[ii*ps1+jj] = r < p->makekernel ? s[i*ps1+j] : 0; /*printf("(%zu, %zu) --> (%zu, %zu)\n", i, j, ii, jj);*/ } } /* Divide all elements by the sum so the kernel is normalized: */ df=(d=n)+ps0*ps1; do *d++/=sum; while(d<df); /* Clean up: */ free(s); *spatial=n; } /******************************************************************/ /************* Frequency domain convolution *****************/ /******************************************************************/ /* The indexs array specifies the row or column numbers for this thread to work on. If forward1backwardn1 is one, then this is the forward transform, meaning that in convolution there are two images. If it is -1, then this is the final backward transform and there is only one image to run FFTW on and the values in indexs will always be smaller than p->s0 and p->s1. When there are two images, then the index numbers are going to be at most double p->s0 and p->s1. In this case, those index values which are smaller than p->s0 or p->s1 belong to the input image and those which are equal or larger than larger belong to the kernel image (after subtraction for p->s0 or p->s1).*/ void * onedimensionfft(void *inparam) { struct fftonthreadparams *fp = (struct fftonthreadparams *)inparam; struct convolveparams *p=fp->p; double *d, *df; size_t indmultip, maxindex; gsl_fft_complex_workspace *work; gsl_fft_complex_wavetable *wavetable; double *data, *pimg=p->pimg, *pker=p->pker; int forward1backwardn1=fp->forward1backwardn1; size_t i, size, stride=fp->stride, *indexs=fp->indexs; /* Set the number of points to transform, indmultip: The value to be multiplied by the value in indexs to specify the first pixel of the row or column. */ if(stride==1) { size=p->ps1; wavetable=fp->ps1wave; work=fp->ps1work; maxindex=p->ps0; indmultip=p->ps1; } else { size=p->ps0; wavetable=fp->ps0wave; work=fp->ps0work; maxindex=p->ps1; indmultip=1; } /* Go over all the rows or columns given for this thread. NOTE: The final array (after the two FFT'd arrays are multiplied by each other) is stored in p->pimg. So the check below works both in the forward and the backward transformation. */ for(i=0; indexs[i]!=GAL_BLANK_SIZE_T; ++i) { data = ( indexs[i]<maxindex ? &pimg[ 2*indexs[i]*indmultip ] /* *2 because complex. */ : &pker[ 2*(indexs[i]-maxindex)*indmultip ] ); gsl_fft_complex_transform(data, stride, size, wavetable, work, forward1backwardn1); /* Normalize in the backward transform: */ if(forward1backwardn1==-1) { df=(d=data)+2*size*stride; do {*d/=size; *(d+1)/=size; d+=2*stride;} while(d<df); } } /* Wait until all other threads finish. */ if(p->cp.numthreads>1) pthread_barrier_wait(fp->b); return NULL; } /* Do the forward Fast Fourier Transform either on two input images (the padded image and kernel) or on one image (the multiplication of the FFT of the two). In the second case, it is assumed that we are looking at the complex conjugate of the array so in practice this will be a backward transform. */ void twodimensionfft(struct convolveparams *p, struct fftonthreadparams *fp, int forward1backwardn1) { int err; pthread_t t; /* All thread ids saved in this, not used. */ pthread_attr_t attr; pthread_barrier_t b; size_t i, nb, *indexs, thrdcols; size_t nt=p->cp.numthreads, multiple=0; /* First we are going to get the 1D fourier transform on the rows of both images. */ if(forward1backwardn1==1) multiple=2; else if(forward1backwardn1==-1) multiple=1; else error(EXIT_FAILURE, 0, "%s: a bug! The value of the variable " "`forward1backwardn1' is %d not 1 or 2. Please contact us at %s " "so we can find the cause of the problem and fix it", __func__, forward1backwardn1, PACKAGE_BUGREPORT); /* ==================== */ /* 1D FFT on each row. */ /* ==================== */ gal_threads_dist_in_threads(multiple*p->ps0, nt, &indexs, &thrdcols); if(nt==1) { fp[0].stride=1; fp[0].indexs=&indexs[0]; fp[0].forward1backwardn1=forward1backwardn1; onedimensionfft(&fp[0]); } else { /* Initialize the attributes. Note that this running thread (that spinns off the nt threads) is also a thread, so the number the barrier should be one more than the number of threads spinned off. */ if( multiple*p->ps0 < nt ) nb=multiple*p->ps0+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); /* Spin off the threads: */ for(i=0;i<nt;++i) if(indexs[i*thrdcols]!=GAL_BLANK_SIZE_T) { fp[i].id=i; fp[i].b=&b; fp[i].stride=1; /* On each row, stride=1 */ fp[i].indexs=&indexs[i*thrdcols]; fp[i].forward1backwardn1=forward1backwardn1; err=pthread_create(&t, &attr, onedimensionfft, &fp[i]); if(err) error(EXIT_FAILURE, 0, "%s: can't create thread %zu for rows", __func__, i); } /* Wait for all threads to finish and free the spaces. */ pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } free(indexs); /* ====================== */ /* 1D FFT on each column. */ /* ====================== */ /* No comments, exact duplicate, except the p->ps1s! */ gal_threads_dist_in_threads(multiple*p->ps1, nt, &indexs, &thrdcols); if(nt==1) { fp[0].stride=p->ps1; fp[0].indexs=indexs; fp[0].forward1backwardn1=forward1backwardn1; onedimensionfft(&fp[0]); } else { if( multiple*p->ps1 < nt ) nb=multiple*p->ps1+1; else nb=nt+1; gal_threads_attr_barrier_init(&attr, &b, nb); for(i=0;i<nt;++i) if(indexs[i*thrdcols]!=GAL_BLANK_SIZE_T) { fp[i].b=&b; fp[i].stride=p->ps1; /* On each column, stride is p->ps1 */ fp[i].indexs=&indexs[i*thrdcols]; fp[i].forward1backwardn1=forward1backwardn1; err=pthread_create(&t, &attr, onedimensionfft, &fp[i]); if(err) error(EXIT_FAILURE, 0, "%s: can't create thread %zu for columns", __func__, i); } pthread_barrier_wait(&b); pthread_attr_destroy(&attr); pthread_barrier_destroy(&b); } free(indexs); } void convolve_frequency(struct convolveparams *p) { double *tmp; size_t dsize[2]; struct timeval t1; gal_data_t *data=NULL; struct fftonthreadparams *fp; /* Make the padded arrays. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); frequency_make_padded_complex(p); if(!p->cp.quiet) gal_timing_report(&t1, "Input and Kernel images padded.", 1); if(p->checkfreqsteps) { /* Prepare the data structure for viewing the steps, note that we don't need the array that is initially made. */ dsize[0]=p->ps0; dsize[1]=p->ps1; data=gal_data_alloc(NULL, GAL_TYPE_FLOAT64, 2, dsize, NULL, 0, p->cp.minmapsize, NULL, NULL, NULL); free(data->array); /* Save the padded input image. */ complextoreal(p->pimg, p->ps0*p->ps1, COMPLEX_TO_REAL_REAL, &tmp); data->array=tmp; data->name="input padded"; gal_fits_img_write(data, p->freqstepsname, NULL, PROGRAM_NAME); free(tmp); data->name=NULL; /* Save the padded kernel image. */ complextoreal(p->pker, p->ps0*p->ps1, COMPLEX_TO_REAL_REAL, &tmp); data->array=tmp; data->name="kernel padded"; gal_fits_img_write(data, p->freqstepsname, NULL, PROGRAM_NAME); free(tmp); data->name=NULL; } /* Initialize the structures: */ fftinitializer(p, &fp); /* Forward 2D FFT on each image. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); twodimensionfft(p, fp, 1); if(!p->cp.quiet) gal_timing_report(&t1, "Images converted to frequency domain.", 1); if(p->checkfreqsteps) { complextoreal(p->pimg, p->ps0*p->ps1, COMPLEX_TO_REAL_SPEC, &tmp); data->array=tmp; data->name="input transformed"; gal_fits_img_write(data, p->freqstepsname, NULL, PROGRAM_NAME); free(tmp); data->name=NULL; complextoreal(p->pker, p->ps0*p->ps1, COMPLEX_TO_REAL_SPEC, &tmp); data->array=tmp; data->name="kernel transformed"; gal_fits_img_write(data, p->freqstepsname, NULL, PROGRAM_NAME); free(tmp); data->name=NULL; } /* Multiply or divide the two arrays and save them in the output.*/ if(!p->cp.quiet) gettimeofday(&t1, NULL); if(p->makekernel) { complexarraydivide(p->pimg, p->pker, p->ps0*p->ps1, p->minsharpspec); if(!p->cp.quiet) gal_timing_report(&t1, "Divided in the frequency domain.", 1); } else { complexarraymultiply(p->pimg, p->pker, p->ps0*p->ps1); if(!p->cp.quiet) gal_timing_report(&t1, "Multiplied in the frequency domain.", 1); } if(p->checkfreqsteps) { complextoreal(p->pimg, p->ps0*p->ps1, COMPLEX_TO_REAL_SPEC, &tmp); data->array=tmp; data->name=p->makekernel ? "Divided" : "Multiplied"; gal_fits_img_write(data, p->freqstepsname, NULL, PROGRAM_NAME); free(tmp); data->name=NULL; } /* Forward (in practice inverse) 2D FFT on each image. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); twodimensionfft(p, fp, -1); if(p->makekernel) correctdeconvolve(p, &p->rpad); else complextoreal(p->pimg, p->ps0*p->ps1, COMPLEX_TO_REAL_REAL, &p->rpad); if(!p->cp.quiet) gal_timing_report(&t1, "Converted back to the spatial domain.", 1); if(p->checkfreqsteps) { data->array=p->rpad; data->name="padded output"; gal_fits_img_write(data, p->freqstepsname, NULL, PROGRAM_NAME); data->name=NULL; data->array=NULL; } /* Free the padded arrays (they are no longer needed) and put the converted array (that is real, not complex) in p->pimg. */ gal_data_free(data); free(p->pimg); free(p->pker); /* Crop out the center, numbers smaller than 10^{-17} are errors, remove them. */ if(!p->cp.quiet) gettimeofday(&t1, NULL); removepaddingcorrectroundoff(p); if(!p->cp.quiet) gal_timing_report(&t1, "Padded parts removed.", 1); /* Free all the allocated space. */ freefp(fp); } /******************************************************************/ /************* Outside function *****************/ /******************************************************************/ void convolve(struct convolveparams *p) { gal_data_t *out, *check; struct gal_options_common_params *cp=&p->cp; /* Do the convolution. */ if(p->domain==CONVOLVE_DOMAIN_SPATIAL) { /* Prepare the mesh structure. */ gal_tile_full_two_layers(p->input, &cp->tl); /* Save the tile IDs if they are requested. */ if(cp->tl.tilecheckname) { check=gal_tile_block_check_tiles(cp->tl.tiles); gal_fits_img_write(check, cp->tl.tilecheckname, NULL, PROGRAM_NAME); gal_data_free(check); } /* Do the spatial convolution. One of the main reason someone would want to do spatial domain convolution with this Convolve program is edge correction. So by default we assume it and will only ignore it if the user asks.*/ out=gal_convolve_spatial(cp->tl.tiles, p->kernel, cp->numthreads, !p->noedgecorrection, cp->tl.workoverch); /* Clean up: free the actual input and replace it's pointer with the convolved dataset to save as output. */ gal_tile_full_free_contents(&cp->tl); gal_data_free(p->input); p->input=out; } else convolve_frequency(p); /* Save the output (which is in p->input) array. */ gal_fits_img_write_to_type(p->input, cp->output, NULL, PROGRAM_NAME, cp->type); } ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/ui.c����������������������������������������������������������������������0000644�0001750�0001750�00000041556�13216276304�013344� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/tile.h> #include <gnuastro/blank.h> #include <gnuastro/table.h> #include <gnuastro/threads.h> #include <gnuastro/arithmetic.h> #include <gnuastro/statistics.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will convolve an input " "image with a given spatial kernel (image) in the spatial domain (no " "edge effects) or frequency domain. The latter suffers from edge effects, " "but can be much faster.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct convolveparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->program_struct = p; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->poptions = program_options; cp->numthreads = gal_threads_number(); cp->coptions = gal_commonopts_options; /* Set the mandatory common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: case GAL_OPTIONS_KEY_TABLEFORMAT: case GAL_OPTIONS_KEY_INTERPNUMNGB: case GAL_OPTIONS_KEY_INTERPONLYBLANK: cp->coptions[i].flags=OPTION_HIDDEN; break; } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct convolveparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: if(p->filename) argp_error(state, "only one argument (input file) should be given"); else p->filename=arg; break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ static void ui_read_check_only_options(struct convolveparams *p) { struct gal_options_common_params *cp=&p->cp; /* Make sure the kernel name is a FITS file and a HDU is given. */ if( gal_fits_name_is_fits(p->kernelname)==0 ) error(EXIT_FAILURE, 0, "`%s' is not a recognized FITS file name", p->kernelname); /* Read the domain from a string into an integer. */ if( !strcmp("spatial", p->domainstr) ) p->domain=CONVOLVE_DOMAIN_SPATIAL; else if( !strcmp("frequency", p->domainstr) ) p->domain=CONVOLVE_DOMAIN_FREQUENCY; else error(EXIT_FAILURE, 0, "domain value `%s' not recognized. Please use " "either `spatial' or `frequency'", p->domainstr); /* If we are in the spatial domain, make sure that the necessary parameters are set. */ if( p->domain==CONVOLVE_DOMAIN_SPATIAL ) if( cp->tl.tilesize==NULL || cp->tl.numchannels==NULL ) { if( cp->tl.tilesize==NULL && cp->tl.numchannels==NULL ) error(EXIT_FAILURE, 0, "in spatial convolution, `--numchannels' " "and `--tilesize' are mandatory"); else error(EXIT_FAILURE, 0, "in spatial convolution, `--%s' is " "mandatory: you should use it to set the %s", cp->tl.tilesize ? "numchannels" : "tilesize", ( cp->tl.tilesize ? "number of channels along each dimension of the input" : "size of tiles to cover the input along each " "dimension" ) ); } } static void ui_check_options_and_arguments(struct convolveparams *p) { /* Make sure an input file name was given and if it was a FITS file, that a HDU is also given. */ if(p->filename==NULL) error(EXIT_FAILURE, 0, "no input file is specified"); /* Make sure the input name is a FITS file name. */ if( gal_fits_name_is_fits(p->filename)==0 ) error(EXIT_FAILURE, 0, "`%s' is not a recognized FITS file name", p->filename); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ /* Read the kernel. VERY IMPORTANT: We can't use the `fits_img_read_kernel' because the Convolve program also does de-convolution. */ static void ui_read_kernel(struct convolveparams *p) { float *f, *ff; /* Read the image into file. */ p->kernel = gal_fits_img_read_to_type(p->kernelname, p->khdu, GAL_TYPE_FLOAT32, p->cp.minmapsize, 0, 0); if(p->kernel->wcs) { wcsfree(p->kernel->wcs); p->kernel->wcs=NULL; } /* Convert all the NaN pixels to zero if the kernel contains blank pixels, also update the flags so it is not checked any more. */ if(gal_blank_present(p->kernel, 1)) { ff = (f=p->kernel->array) + p->kernel->size; do *f = isnan(*f) ? 0.0f : *f; while(++f<ff); p->kernel->flag |= GAL_DATA_FLAG_BLANK_CH; p->kernel->flag &= ~GAL_DATA_FLAG_HASBLANK; } } static void ui_preparations(struct convolveparams *p) { size_t i, size; gal_data_t *sum; float *kernel, tmp; struct gal_options_common_params *cp=&p->cp; char *outsuffix = p->makekernel ? "_kernel.fits" : "_convolved.fits"; /* Set the output name if the user hasn't set it. */ if(cp->output==NULL) cp->output=gal_checkset_automatic_output(cp, p->filename, outsuffix); gal_checkset_writable_remove(cp->output, 0, cp->dontdelete); if(p->checkfreqsteps) { p->freqstepsname=gal_checkset_automatic_output(cp, p->filename, "_freqsteps.fits"); gal_checkset_writable_remove(p->freqstepsname, 0, cp->dontdelete); } if(cp->tl.checktiles) { cp->tl.tilecheckname=gal_checkset_automatic_output(cp, p->filename, "_tiled.fits"); gal_checkset_writable_remove(cp->tl.tilecheckname, 0, cp->dontdelete); } /* Read the input image as a float64 array. */ p->input=gal_fits_img_read_to_type(p->filename, cp->hdu, GAL_TYPE_FLOAT32, cp->minmapsize, 0, 0); /* Currently Convolve only works on 2D images. */ if(p->input->ndim!=2) error(EXIT_FAILURE, 0, "%s (hdu %s) has %zu dimensions. Currently " "Convolve only operates on 2D images", p->filename, cp->hdu, p->input->ndim); /* See if there are any blank values. */ if(p->domain==CONVOLVE_DOMAIN_FREQUENCY) { if( gal_blank_present(p->input, 1) ) fprintf(stderr, "\n----------------------------------------\n" "######## %s WARNING ########\n" "There are blank pixels in `%s' (hdu: `%s') and you have " "asked for frequency domain convolution. As a result, all " "the pixels in the output (`%s') will be blank. Only " "spatial domain convolution can account for blank pixels " "in the input data. You can run %s again with " "`--domain=spatial'\n" "----------------------------------------\n\n", PROGRAM_NAME, p->filename, cp->hdu, cp->output, PROGRAM_NAME); } else gal_tile_full_sanity_check(p->filename, cp->hdu, p->input, &cp->tl); /* Read the file specified by --kernel. If makekernel is specified, then this is actually the sharper image and the input image (given as an argument) is the blurry image. */ if(p->makekernel) { /* Read in the kernel array. */ ui_read_kernel(p); /* Make sure the size of the kernel is the same as the input */ if( p->input->dsize[0]!=p->kernel->dsize[0] || p->input->dsize[1]!=p->kernel->dsize[1] ) error(EXIT_FAILURE, 0, "with the `--makekernel' (`-m') option, " "the input image and the image specified with the `--kernel' " "(`-k') option should have the same size. The lower resolution " "input image (%s) has %zux%zu pixels while the sharper image " "(%s) specified with the kernel option has %zux%zu pixels", p->filename, p->input->dsize[1], p->input->dsize[0], p->kernelname, p->kernel->dsize[1], p->kernel->dsize[0]); /* Divide both images by their sum so their lowest frequency becomes 1 and their division (in the frequency domain) would be meaningful. */ sum=gal_statistics_sum(p->input); sum=gal_data_copy_to_new_type_free(sum, GAL_TYPE_FLOAT32); p->input = gal_arithmetic(GAL_ARITHMETIC_OP_DIVIDE, GAL_ARITHMETIC_FLAGS_ALL, p->input, sum); sum=gal_statistics_sum(p->kernel); sum=gal_data_copy_to_new_type_free(sum, GAL_TYPE_FLOAT32); p->kernel = gal_arithmetic(GAL_ARITHMETIC_OP_DIVIDE, GAL_ARITHMETIC_FLAGS_ALL, p->kernel, sum); } /* Read the kernel. If there is anything particular to Convolve, then don't use the standard kernel reading function in fits.c. Otherwise just use the same one that all programs use. The standard one is faster because it mixes the NaN conversion and also the normalization into one loop. */ else { if(p->nokernelnorm || p->nokernelflip) { /* Read in the kernel array: */ ui_read_kernel(p); /* Check its size (must be odd). */ if(p->kernel->dsize[0]%2==0 || p->kernel->dsize[1]%2==0) error(EXIT_FAILURE, 0, "the kernel image has to have an odd " "number of pixels on both sides (there has to be on pixel " "in the center). %s (hdu: %s) is %zu by %zu", p->kernelname, p->khdu, p->kernel->dsize[1], p->kernel->dsize[0]); /* Normalize the kernel: */ if( !p->nokernelnorm ) { sum=gal_statistics_sum(p->kernel); p->kernel = gal_arithmetic(GAL_ARITHMETIC_OP_DIVIDE, GAL_ARITHMETIC_FLAGS_ALL, p->kernel, sum); } /* Flip the kernel: */ if( !p->nokernelflip ) { size=p->kernel->size; kernel=p->kernel->array; for(i=0;i<p->kernel->size/2;++i) { tmp = kernel[ i ]; kernel[ i ] = kernel[ size - i - 1 ]; kernel[ size - i - 1 ] = tmp; } } } else p->kernel = gal_fits_img_read_kernel(p->kernelname, p->khdu, cp->minmapsize); } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ static void ui_print_intro(struct convolveparams *p) { printf("%s started on %s", PROGRAM_NAME, ctime(&p->rawtime)); printf(" - Using %zu CPU threads.\n", p->cp.numthreads); printf(" - Input: %s (hdu: %s)\n", p->filename, p->cp.hdu); printf(" - Kernel: %s (hdu: %s)\n", p->kernelname, p->khdu); } void ui_read_check_inputs_setup(int argc, char *argv[], struct convolveparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Do a sanity check only on options. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); /* Everything is ready, print the intro if not in quiet mode. */ if(!p->cp.quiet) ui_print_intro(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct convolveparams *p, struct timeval *t1) { /* Free the allocated arrays: */ free(p->khdu); free(p->cp.hdu); free(p->cp.output); gal_data_free(p->input); gal_data_free(p->kernel); /* Print the final message. */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in: ", 0); } ��������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/main.c��������������������������������������������������������������������0000644�0001750�0001750�00000003127�13121462410�013631� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Convolve - Convolve input data with a given kernel. Convolve is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "convolve.h" #include "ui.h" /* Needs convolveparams in main.h */ int main(int argc, char *argv[]) { struct timeval t1; struct convolveparams p={{{0},0},0}; /* Set the starting time.*/ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run Image Crop */ convolve(&p); /* Free all non-freed allocations. */ ui_free_report(&p, &t1); /* Return successfully. */ return EXIT_SUCCESS; } 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= @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINDOWS_STAT_INODES = @WINDOWS_STAT_INODES@ WINDOWS_STAT_TIMESPEC = @WINDOWS_STAT_TIMESPEC@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = @abs_top_srcdir@ ac_ct_AR = @ac_ct_AR@ ac_ct_CC = @ac_ct_CC@ ac_ct_CXX = @ac_ct_CXX@ ac_ct_DUMPBIN = @ac_ct_DUMPBIN@ am__include = @am__include@ am__leading_dot = @am__leading_dot@ am__quote = @am__quote@ am__tar = @am__tar@ am__untar = @am__untar@ ax_pthread_config = @ax_pthread_config@ bindir = @bindir@ build = @build@ build_alias = @build_alias@ build_cpu = @build_cpu@ build_os = @build_os@ build_vendor = @build_vendor@ builddir = @builddir@ datadir = @datadir@ datarootdir = @datarootdir@ docdir = @docdir@ dvidir = @dvidir@ exec_prefix = @exec_prefix@ gl_LIBOBJS = @gl_LIBOBJS@ gl_LTLIBOBJS = @gl_LTLIBOBJS@ gltests_LIBOBJS = @gltests_LIBOBJS@ gltests_LTLIBOBJS = @gltests_LTLIBOBJS@ gltests_WITNESS = @gltests_WITNESS@ has_ghostscript = @has_ghostscript@ has_glibtool = @has_glibtool@ has_help2man = @has_help2man@ has_libtool = @has_libtool@ host = @host@ host_alias = @host_alias@ host_cpu = @host_cpu@ host_os = @host_os@ host_vendor = @host_vendor@ htmldir = @htmldir@ includedir = 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Convolve. # Convolve is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astconvolve --help # Full list of options, short doc. # $ astconvolve -P # Print all options and used values. # $ info astconvolve # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. # Input: kernel kernel.fits khdu 1 # Output: type float32 # Operating mode: domain frequency minsharpspec 0.005 �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convolve/Makefile.am���������������������������������������������������������������0000644�0001750�0001750�00000002602�13121462410�014572� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astconvolve astconvolve_LDADD = -lgnuastro astconvolve_SOURCES = main.c ui.c convolve.c EXTRA_DIST = main.h authors-cite.h args.h ui.h convolve.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astconvolve.conf ������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/��������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�012640� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/jpeg.h��������������������������������������������������������������������0000644�0001750�0001750�00000002310�13121462410�013641� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef JPEG_H #define JPEG_H int nameisjpeg(char *name); int nameisjpegsuffix(char *name); size_t jpeg_read_to_ll(char *filename, gal_data_t **list, size_t minmapsize); void jpeg_write(struct converttparams *p); #endif ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/eps.h���������������������������������������������������������������������0000644�0001750�0001750�00000002275�13121462410�013515� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef EPS_H #define EPS_H int nameiseps(char *name); int nameisepssuffix(char *name); int nameispdf(char *name); int nameispdfsuffix(char *name); void eps_write_eps_or_pdf(struct converttparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/convertt.h����������������������������������������������������������������0000644�0001750�0001750�00000002077�12616616510�014604� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef CONVERTT_H #define CONVERTT_H void convertt(struct converttparams *p); #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/ui.h����������������������������������������������������������������������0000644�0001750�0001750�00000004031�13174462540�013347� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Option groups particular to this program */ enum program_args_groups { UI_GROUP_FLUX = GAL_OPTIONS_GROUP_AFTER_COMMON, }; /* Available letters for short options: a d e f g j k l n p r s t v y z E G J O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_QUALITY = 'u', UI_KEY_WIDTHINCM = 'w', UI_KEY_BORDERWIDTH = 'b', UI_KEY_HEX = 'x', UI_KEY_FLUXLOW = 'L', UI_KEY_FLUXHIGH = 'H', UI_KEY_MAXBYTE = 'm', UI_KEY_FLMINBYTE = 'A', UI_KEY_FHMAXBYTE = 'B', UI_KEY_CHANGE = 'c', UI_KEY_CHANGEAFTERTRUNC = 'C', UI_KEY_INVERT = 'i', /* Only with long version (start with a value 1000, the rest will be set automatically). */ }; void ui_read_check_inputs_setup(int argc, char *argv[], struct converttparams *p); void ui_free_report(struct converttparams *p); #endif �������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/args.h��������������������������������������������������������������������0000644�0001750�0001750�00000012100�13174462540�013662� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { /* Output */ { "quality", UI_KEY_QUALITY, "INT", 0, "Quality of output JPEG image (1 to 100).", GAL_OPTIONS_GROUP_OUTPUT, &p->quality, GAL_TYPE_UINT8, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "widthincm", UI_KEY_WIDTHINCM, "FLT", 0, "Width in units of centimeters.", GAL_OPTIONS_GROUP_OUTPUT, &p->widthincm, GAL_TYPE_FLOAT32, GAL_OPTIONS_RANGE_GT_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "borderwidth", UI_KEY_BORDERWIDTH, "INT", 0, "EPS/PDF border width in units of 1/72 inch.", GAL_OPTIONS_GROUP_OUTPUT, &p->borderwidth, GAL_TYPE_UINT32, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "hex", UI_KEY_HEX, 0, 0, "Hexadecimal encoding in EPS. Default: ASCII85.", GAL_OPTIONS_GROUP_OUTPUT, &p->hex, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { 0, 0, 0, 0, "Flux:", UI_GROUP_FLUX }, { "fluxlow", UI_KEY_FLUXLOW, "FLT", 0, "Lower flux truncation value.", UI_GROUP_FLUX, &p->fluxlowstr, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "fluxhigh", UI_KEY_FLUXHIGH, "FLT", 0, "Higher flux truncation value.", UI_GROUP_FLUX, &p->fluxhighstr, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "maxbyte", UI_KEY_MAXBYTE, "INT", 0, "Maximum byte value for all color channels.", UI_GROUP_FLUX, &p->maxbyte, GAL_TYPE_UINT8, GAL_OPTIONS_RANGE_GE_0, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "flminbyte", UI_KEY_FLMINBYTE, 0, 0, "Set value of fluxlow as the minimum byte value.", UI_GROUP_FLUX, &p->flminbyte, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "fhmaxbyte", UI_KEY_FHMAXBYTE, 0, 0, "Set value of fluxhigh as the maximum byte value.", UI_GROUP_FLUX, &p->fhmaxbyte, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "change", UI_KEY_CHANGE, "STR", 0, "Change pixel values `from_1:to_1,from_2:to_2`.", UI_GROUP_FLUX, &p->changestr, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "changeaftertrunc", UI_KEY_CHANGEAFTERTRUNC, 0, 0, "First truncate then change pixel values.", UI_GROUP_FLUX, &p->changeaftertrunc, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "invert", UI_KEY_INVERT, 0, 0, "Invert the values in JPEG and EPS/PDF.", UI_GROUP_FLUX, &p->invert, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/authors-cite.h������������������������������������������������������������0000644�0001750�0001750�00000002776�13211076737�015360� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ��gnuastro-0.5/bin/convertt/main.h��������������������������������������������������������������������0000644�0001750�0001750�00000006615�13121462410�013654� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "ConvertType" /* Program full name. */ #define PROGRAM_EXEC "astconvertt" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Constants/macros. */ #define BLANK_CHANNEL_NAME "blank" enum output_formats { OUT_FORMAT_INVALID, /* ==0 by C standard */ OUT_FORMAT_TXT, OUT_FORMAT_EPS, OUT_FORMAT_PDF, OUT_FORMAT_FITS, OUT_FORMAT_JPEG, }; /* This is used in converting certain values in the array. */ struct change { gal_data_t *from; gal_data_t *to; struct change *next; }; struct converttparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ gal_list_str_t *inputnames; /* The names of input files. */ gal_list_str_t *hdus; /* The names of input hdus. */ uint8_t quality; /* Quality of JPEG image. */ float widthincm; /* Width in centimeters. */ uint32_t borderwidth; /* Width of border in PostScript points. */ uint8_t hex; /* Use hexadecimal not ASCII85 encoding. */ char *fluxlowstr; /* Lower flux truncation value. */ char *fluxhighstr; /* Higher flux truncation value. */ uint8_t maxbyte; /* Maximum byte value. */ uint8_t flminbyte; /* fluxlow is minimum byte. */ uint8_t fhmaxbyte; /* fluxhigh is maximum byte. */ char *changestr; /* String of change values. */ uint8_t changeaftertrunc; /* First convert, then truncate. */ uint8_t invert; /* ==1: invert the output image. */ /* Internal */ struct change *change; /* The value conversion string. */ gal_data_t *fluxlow; /* The lower flux truncation. */ gal_data_t *fluxhigh; /* The higher flux truncation. */ time_t rawtime; /* Starting time of the program. */ int outformat; /* The format of the output file. */ size_t numch; /* Current Channel. */ gal_data_t *chll; /* Linked list of color channels. */ }; #endif �������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/jpeg.c��������������������������������������������������������������������0000644�0001750�0001750�00000024407�13121462410�013647� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <setjmp.h> #include <string.h> #ifdef HAVE_LIBJPEG #include <jpeglib.h> #endif #include <gnuastro/list.h> #include <gnuastro/fits.h> #include "main.h" #include "jpeg.h" /************************************************************* ************** Acceptable JPEG names ************** *************************************************************/ int nameisjpeg(char *name) { size_t len; len=strlen(name); if ( ( len>=3 && strcmp(&name[len-3], "jpg") == 0 ) || ( len>=3 && strcmp(&name[len-3], "JPG") == 0 ) || ( len>=4 && strcmp(&name[len-4], "jpeg") == 0 ) || ( len>=4 && strcmp(&name[len-4], "JPEG") == 0 ) || ( len>=3 && strcmp(&name[len-3], "jpe") == 0 ) || ( len>=3 && strcmp(&name[len-3], "jif") == 0 ) || ( len>=4 && strcmp(&name[len-4], "jfif") == 0 ) || ( len>=3 && strcmp(&name[len-3], "jfi") == 0 ) ) return 1; else return 0; } int nameisjpegsuffix(char *name) { if (strcmp(name, "jpg") == 0 || strcmp(name, ".jpg") == 0 || strcmp(name, "JPG") == 0 || strcmp(name, ".JPG") == 0 || strcmp(name, "jpeg") == 0 || strcmp(name, ".jpeg") == 0 || strcmp(name, "JPEG") == 0 || strcmp(name, ".JPEG") == 0 || strcmp(name, "jpe") == 0 || strcmp(name, ".jpe") == 0 || strcmp(name, "jif") == 0 || strcmp(name, ".jif") == 0 || strcmp(name, "jfif") == 0 || strcmp(name, ".jfif") == 0 || strcmp(name, "jfi") == 0 || strcmp(name, ".jfi") == 0) return 1; else return 0; } #ifdef HAVE_LIBJPEG /************************************************************* ************** Read a JPEG image ************** *************************************************************/ /* Read the example.c in libjpeg's source code to understand the details of what is going on here. */ struct my_error_mgr { struct jpeg_error_mgr pub; /* "public" fields */ jmp_buf setjmp_buffer; /* for return to caller */ }; typedef struct my_error_mgr *my_error_ptr; METHODDEF(void) jpeg_error_exit(j_common_ptr cinfo) { /* cinfo->err really points to a my_error_mgr struct, so coerce pointer */ my_error_ptr myerr = (my_error_ptr) cinfo->err; /* Always display the message. */ /* We could postpone this until after returning, if we chose. */ (*cinfo->err->output_message) (cinfo); /* Return control to the setjmp point */ longjmp(myerr->setjmp_buffer, 1); } void makejsample(JSAMPLE **a, size_t size) { JSAMPLE *jsarr; if(sizeof *jsarr!=1) { printf("\n\nJSAMPLE has to be unsigned char!\n\n"); exit(EXIT_FAILURE); } errno=0; jsarr=malloc(size*sizeof *jsarr); if(jsarr==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for jsarr", __func__, size*sizeof *jsarr); *a=jsarr; } unsigned char ** readjpg(char *inname, size_t *outs0, size_t *outs1, size_t *numcolors) { FILE * infile; JSAMPROW jrow; JSAMPLE *jsamp; int rowstride, c; JSAMPARRAY jsarr; unsigned char **all; struct my_error_mgr jerr; size_t i, j, size, nc, s0, s1; struct jpeg_decompress_struct cinfo; /* Open the input file */ errno=0; if ((infile = fopen(inname, "rb")) == NULL) error(EXIT_FAILURE, errno, "%s", inname); /* Set up the error and decompressing (reading) functions. */ cinfo.err = jpeg_std_error(&jerr.pub); jerr.pub.error_exit = jpeg_error_exit; if (setjmp(jerr.setjmp_buffer)) { jpeg_destroy_decompress(&cinfo); fclose(infile); error(EXIT_FAILURE, 0, "%s: problem in reading %s", __func__, inname); } jpeg_create_decompress(&cinfo); jpeg_stdio_src(&cinfo, infile); /* Read the JPEG header information and start de-compressing: */ jpeg_read_header(&cinfo, TRUE); jpeg_start_decompress(&cinfo); /* Get the array width and height and number of color channels: */ s0=*outs0=cinfo.output_height; s1=*outs1=cinfo.output_width; size=s0*s1; nc=*numcolors=cinfo.output_components; rowstride=s1*nc; makejsample(&jsamp, size*nc); /* Allocate all the arrays for each color: */ errno=0; all=malloc(nc*sizeof *all); if(all==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `all'", __func__, nc*sizeof *all); for(i=0;i<nc;++i) { errno=0; all[i]=malloc(s0*s1*sizeof *all[i]); if(all[i]==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `all[%zu]'", __func__, s0*s1*sizeof *all[i], i); } /* Read the image line by line: */ c=s0-1; while (cinfo.output_scanline < cinfo.output_height) { jrow=&jsamp[c-- * rowstride]; jsarr=&jrow; jpeg_read_scanlines(&cinfo, jsarr, 1); } /* Put the different colors into the different arrays */ for(i=0;i<size;++i) for(j=0;j<nc;++j) all[j][i]=jsamp[i*nc+j]; /* Finish decompression, destroy it and close file: */ jpeg_finish_decompress(&cinfo); jpeg_destroy_decompress(&cinfo); fclose(infile); free(jsamp); return all; } /* Read each color channel of a JPEG image as a separate array and put them in a linked list of data-structures. */ size_t jpeg_read_to_ll(char *filename, gal_data_t **list, size_t minmapsize) { char *name; size_t ndim=2, dsize[2]; unsigned char **allcolors; size_t i, s0, s1, numcolors; /* Read the JPEG image into the all array. */ allcolors=readjpg(filename, &s0, &s1, &numcolors); /* Add the arrays to the linked list. */ for(i=0;i<numcolors;++i) { dsize[0]=s0; dsize[1]=s1; asprintf(&name, "JPEG_CH_%zu", i+1); gal_list_data_add_alloc(list, allcolors[i], GAL_TYPE_UINT8, ndim, dsize, NULL, 0, minmapsize, name, NULL, NULL); free(name); } /* Free the array keeping the pointers to each channel. Note that each channel was allocated separately and goes out of this function with the data structure, so we just have to free the outer array that kept all the channels. */ free(allcolors); /* Return the number of color channels. */ return numcolors; } /************************************************************* ************** Write a JPEG image ************** *************************************************************/ static void jpeg_write_array(JSAMPLE *jsr, struct converttparams *p) { JSAMPROW r[1]; FILE * outfile; int row_stride=0, c; struct jpeg_error_mgr jerr; size_t *dsize=p->chll->dsize; struct jpeg_compress_struct cinfo; /* Begin the JPEG writing, following libjpeg's example.c */ cinfo.err = jpeg_std_error(&jerr); jpeg_create_compress(&cinfo); errno=0; if ((outfile = fopen(p->cp.output, "wb")) == NULL) error(EXIT_FAILURE, errno, "%s", p->cp.output); jpeg_stdio_dest(&cinfo, outfile); cinfo.image_width = dsize[1]; cinfo.image_height = dsize[0]; switch(p->numch) { case 1: row_stride=dsize[1]; cinfo.input_components = 1; cinfo.in_color_space = JCS_GRAYSCALE; break; case 3: row_stride=3*dsize[1]; cinfo.input_components = 3; cinfo.in_color_space = JCS_RGB; break; case 4: row_stride=4*dsize[1]; cinfo.input_components = 4; cinfo.in_color_space = JCS_CMYK; break; default: error(EXIT_FAILURE, 0, "%s: a bug! The number of channels is not 1, 3 " "or 4, but %zu. This should not happen. Please contact us so we " "can fix the problem", __func__, p->numch); } jpeg_set_defaults(&cinfo); jpeg_set_quality(&cinfo, p->quality, TRUE); cinfo.density_unit=1; cinfo.Y_density=cinfo.X_density=dsize[1]/(p->widthincm/2.54); jpeg_start_compress(&cinfo, TRUE); /* cinfo.next_scanline is 'unsigned int' */ c=dsize[0]-1; /* In JPEG the first row is on the bottom! */ while (cinfo.next_scanline < cinfo.image_height) { r[0] = & jsr[c-- * row_stride]; (void) jpeg_write_scanlines(&cinfo, r, 1); } jpeg_finish_compress(&cinfo); fclose(outfile); jpeg_destroy_compress(&cinfo); } void jpeg_write(struct converttparams *p) { JSAMPLE *jsr; gal_data_t *channel; unsigned char *colors[4]; size_t i, pixel, color, numch=p->numch; /* A small sanity check */ if(p->numch==2 || p->numch>4) error(EXIT_FAILURE, 0, "%s: only 1, 3, and 4 color channels are " "acceptable", __func__); /* Make sure the JSAMPLE is 8bits, then allocate the necessary space based on the number of channels. */ if(sizeof *jsr!=1) error(EXIT_FAILURE, 0, "%s: JSAMPLE has to be 8bit", __func__); errno=0; jsr=malloc(numch * p->chll->size * sizeof *jsr); if(jsr==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for jsr", __func__, numch * p->chll->size * sizeof *jsr ); /* Set the pointers to each color. */ i=0; for(channel=p->chll; channel!=NULL; channel=channel->next) colors[i++]=channel->array; /* Write the different colors into jsr. */ for(pixel=0; pixel<p->chll->size; ++pixel) for(color=0;color<numch;++color) { jsr[pixel*numch+color] = colors[color][pixel]; /* printf("color: %zu, pixel: %zu, jsr: %d\n", color, pixel, (int)jsr[pixel*numch+color]); */ } /* Write jsr to a JPEG image and clean up. */ jpeg_write_array(jsr, p); free(jsr); } #endif /* HAVE_LIBJPEG */ ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/eps.c���������������������������������������������������������������������0000644�0001750�0001750�00000030606�13152356630�013521� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" /************************************************************* ************** Acceptable EPS names *************** *************************************************************/ int nameiseps(char *name) { size_t len; len=strlen(name); if ( ( len>=3 && strcmp(&name[len-3], "eps") == 0 ) || ( len>=3 && strcmp(&name[len-3], "EPS") == 0 ) || ( len>=4 && strcmp(&name[len-4], "epsf") == 0 ) || ( len>=4 && strcmp(&name[len-4], "epsi") == 0 ) ) return 1; else return 0; } int nameisepssuffix(char *name) { if (strcmp(name, "eps") == 0 || strcmp(name, ".eps") == 0 || strcmp(name, "EPS") == 0 || strcmp(name, ".EPS") == 0 || strcmp(name, "epsf") == 0 || strcmp(name, ".epsf") == 0 || strcmp(name, "epsi") == 0 || strcmp(name, ".epsi") == 0) return 1; else return 0; } int nameispdf(char *name) { size_t len; len=strlen(name); if (strcmp(&name[len-3], "pdf") == 0 || strcmp(&name[len-3], "PDF") == 0) return 1; else return 0; } int nameispdfsuffix(char *name) { if (strcmp(name, "pdf") == 0 || strcmp(name, ".pdf") == 0 || strcmp(name, "PDF") == 0 || strcmp(name, ".PDF") == 0) return 1; else return 0; } /************************************************************* ************** Write an EPS image ************** *************************************************************/ static int eps_is_binary(struct converttparams *p) { gal_data_t *channel; unsigned char *i, *fi; /* Go through all the channels. */ for(channel=p->chll; channel!=NULL; channel=channel->next) { /* Go through all the values and see they are 0 and break out of the loop as soon as you get to a pixel that is not 0 or `maxbyte'. */ fi = (i=p->chll->array) + p->chll->size; do if(*i!=p->maxbyte && *i!=0) break; while(++i<fi); /* If we didn't get to the end of the channel, then we have a non-binary image. */ if(i!=fi) return 0; } /* If we get to this point, then all the channels were binary, so return success. */ return 1; } /* Show the bit values in a uint8_t variable. It is included here as a test in debugging problems with blackandwhite. To test it use a very small valued input to make the outputs reasonable. For example I am now testing it with an input text array of 12 elements (while calling the --invert option): 1 0 1 0 0 0 0 0 0 1 0 1 */ void eps_show_bits(uint8_t x) { int i; for(i=7;i>=0;--i) (x&(1<<i)) ? putchar('1') : putchar('0'); putchar('\n'); } /* Convert the channels into into a 0 and 1 bit stream. This function is only called when the image is binary (has only two values). NOTE: each row has to have an integer number of bytes, so when the number of pixels in a row is not a multiple of 8, we'll add one. */ size_t eps_convert_to_bitstream(struct converttparams *p) { gal_data_t *channel; size_t i, j, k, bytesinrow, bytesinimg; unsigned char *bits, byte, curbit, *in; size_t s0=p->chll->dsize[0], s1=p->chll->dsize[1]; /* Find the size values and allocate the array. */ if( s1 % 8 ) bytesinrow = s1/8 + 1; else bytesinrow = s1/8; bytesinimg = bytesinrow*s0; /* Go over all the channels. */ for(channel=p->chll; channel!=NULL; channel=channel->next) { /* Allocate the array. */ bits=gal_data_malloc_array(GAL_TYPE_UINT8, bytesinimg, __func__, "bits"); /* Put the values in. */ in=channel->array; for(i=0;i<s0;++i) { for(j=0;j<bytesinrow;++j) { /* i*s0+j is the byte, not bit position. */ byte=0; /* Set the 8 bits to zero. */ curbit=0x80; /* Current bit position, starting at: */ for(k=0;k<8;++k) { if( j*8+k < s1 ) { if(in[i*s1+j*8+k]) byte |= curbit; curbit >>= 1; } else break; } /*eps_show_bits(byte);*/ bits[i*bytesinrow+j]=byte; } } free(channel->array); channel->array=bits; channel->type=GAL_TYPE_BIT; } /* Return the total number of bytes in the image. */ return bytesinimg; } void eps_write_hex(struct converttparams *p, FILE *fp, size_t size) { unsigned char *in; gal_data_t *channel; size_t i=0, j, elem_for_newline=35; for(channel=p->chll; channel!=NULL; channel=channel->next) { if(channel->status) /* A blank channel has status==1. */ fprintf(fp, "{<00>} %% Channel %zu is blank\n", i); else { in=channel->array; fprintf(fp, "{<"); for(j=0;j<size;++j) { fprintf(fp, "%02X", in[j]); if(j%elem_for_newline==0) fprintf(fp, "\n"); } fprintf(fp, ">}\n"); } ++i; } } void eps_write_ascii85(struct converttparams *p, FILE *fp, size_t size) { unsigned char *in; gal_data_t *channel; uint32_t anint, base; size_t i=0, j, k, elem_for_newline=15; /* 15*5=75 */ for(channel=p->chll; channel!=NULL; channel=channel->next) { if(channel->status) fprintf(fp, "{<00>} %% Channel %zu is blank\n", i); else { in=channel->array; fprintf(fp, "{<~"); for(j=0;j<size;j+=4) { /* This is the last four bytes */ if(size-j<4) { anint=in[j]*256*256*256; if(size-j>1) anint+=in[j+1]*256*256; if(size-j==3) anint+=in[j+2]*256; } else anint=( in[j]*256*256*256 + in[j+1]*256*256 + in[j+2]*256 + in[j+3] ); /* If all four bytes are zero, then just print `z'. */ if(anint==0) fprintf(fp, "z"); else { /* To check, just change the fprintf below to printf: printf("\n\n"); printf("%u %u %u %u\n", in[i], in[i+1], in[i+2], in[i+3]); */ base=85*85*85*85; /* Do the ASCII85 encoding: */ for(k=0;k<5;++k) { fprintf(fp, "%c", anint/base+33); anint%=base; base/=85; } } /* Go to the next line if on the right place: */ if(j%elem_for_newline==0) fprintf(fp, "\n"); } fprintf(fp, "~>}\n"); } ++i; } } static void eps_write_image(struct converttparams *p, FILE *fp) { int bpc=8; size_t i, size, *dsize=p->chll->dsize; /* Set the number of bits per component. */ if( p->numch==1 && eps_is_binary(p) ) { bpc=1; size=eps_convert_to_bitstream(p); } else size=p->chll->size; switch(p->numch) { case 1: fprintf(fp, "/DeviceGray setcolorspace\n"); break; case 3: fprintf(fp, "/DeviceRGB setcolorspace\n"); break; case 4: fprintf(fp, "/DeviceCMYK setcolorspace\n"); break; default: error(EXIT_FAILURE, 0, "%s: a bug! The number of channels (%zu) is not " "1, 3 or 4. Please contact us so we can find the issue and fix it", __func__, p->numch); } fprintf(fp, "<<\n"); fprintf(fp, " /ImageType 1\n"); fprintf(fp, " /Width %zu\n", dsize[1]); fprintf(fp, " /Height %zu\n", dsize[0]); fprintf(fp, " /ImageMatrix [ %zu 0 0 %zu 0 0 ]\n", dsize[1], dsize[0]); fprintf(fp, " /MultipleDataSources true\n"); fprintf(fp, " /BitsPerComponent %d\n", bpc); fprintf(fp, " /Decode["); for(i=0;i<p->numch;++i) {fprintf(fp, " 0 1");} fprintf(fp, " ]\n"); fprintf(fp, " /Interpolate false\n"); fprintf(fp, " /DataSource [\n"); if(p->hex) eps_write_hex(p, fp, size); else eps_write_ascii85(p, fp, size); fprintf(fp, " ]\n"); fprintf(fp, ">>\n"); fprintf(fp, "image\n\n"); } void eps_write_eps_or_pdf(struct converttparams *p) { FILE *fp; float hbw; char command[20000], *epsfilename=NULL; size_t winpt, hinpt, *dsize=p->chll->dsize; /* Find the bounding box */ winpt=p->widthincm*72.0f/2.54f; hinpt=(float)( dsize[0] * winpt )/(float)(dsize[1]); hbw=(float)p->borderwidth/2.0f; /* EPS filename */ if(p->outformat==OUT_FORMAT_EPS) { epsfilename=p->cp.output; gal_checkset_writable_remove(epsfilename, 0, p->cp.dontdelete); } else if (p->outformat==OUT_FORMAT_PDF) { gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); epsfilename=gal_checkset_automatic_output(&p->cp, p->cp.output, ".ps"); } else error(EXIT_FAILURE, 0, "%s: a bug! code %d not recognized for " "`p->outformat'", __func__, p->outformat); /* Open the output file and write the top comments. */ errno=0; fp=fopen(epsfilename, "w"); if(fp==NULL) error(EXIT_FAILURE, errno, "%s", p->cp.output); fprintf(fp, "%%!PS-Adobe-3.0 EPSF-3.0\n"); fprintf(fp, "%%%%BoundingBox: 0 0 %zu %zu\n", winpt+2*p->borderwidth, hinpt+2*p->borderwidth); fprintf(fp, "%%%%Creator: %s\n", PROGRAM_STRING); fprintf(fp, "%%%%CreationDate: %s", ctime(&p->rawtime)); fprintf(fp, "%%%%LanuageLevel: 3\n"); fprintf(fp, "%%%%EndComments\n\n"); if(p->outformat==OUT_FORMAT_EPS) fprintf(fp, "gsave\n\n"); /* Commands to draw the border: */ if(p->borderwidth) { fprintf(fp, "%% Draw the border:\n"); fprintf(fp, "0 setgray\n"); fprintf(fp, "%d setlinewidth\n", p->borderwidth); fprintf(fp, "%.1f %.1f moveto\n", hbw, hbw); fprintf(fp, "0 %zu rlineto\n", hinpt+p->borderwidth); fprintf(fp, "%zu 0 rlineto\n", winpt+p->borderwidth); fprintf(fp, "0 -%zu rlineto\n", hinpt+p->borderwidth); fprintf(fp, "closepath\n"); fprintf(fp, "stroke\n\n"); } /* Write the image: */ fprintf(fp, "%% Draw the image:\n"); fprintf(fp, "%d %d translate\n", p->borderwidth, p->borderwidth); fprintf(fp, "%zu %zu scale\n", winpt, hinpt); eps_write_image(p, fp); /* Ending of the EPS file: */ if(p->outformat==OUT_FORMAT_EPS) fprintf(fp, "grestore\n"); else fprintf(fp, "showpage\n"); fprintf(fp, "%%%%EOF"); fclose(fp); if(p->outformat==OUT_FORMAT_PDF) { sprintf(command, "gs -q -o %s -sDEVICE=pdfwrite -dDEVICEWIDTHPOINTS=%zu" " -dDEVICEHEIGHTPOINTS=%zu -dPDFFitPage %s", p->cp.output, winpt+2*p->borderwidth, hinpt+2*p->borderwidth, epsfilename); if(system(command)) error(EXIT_FAILURE, 0, "the command to convert a PostScript file to " "PDF (`%s') was not successful! The PostScript file (%s) is " "left if you want to convert or use it through any other " "means", command, epsfilename); sprintf(command, "rm %s", epsfilename); if(system(command)) error(EXIT_FAILURE, 0, "The PDF output (%s) was created, but the " "PostScript file which was used to make it (%s) could not be" "removed", p->cp.output, epsfilename); free(epsfilename); } } ��������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/convertt.c����������������������������������������������������������������0000644�0001750�0001750�00000024556�13175442274�014612� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <gnuastro/txt.h> #include <gnuastro/fits.h> #include <gnuastro/arithmetic.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "eps.h" #include "jpeg.h" /**************************************************************/ /************** Modifying pixel values ***************/ /**************************************************************/ static void convertt_change(struct converttparams *p) { gal_data_t *channel, *cond; struct change *change, *tmp; unsigned char flags = ( GAL_ARITHMETIC_NUMOK | GAL_ARITHMETIC_FREE | GAL_ARITHMETIC_INPLACE ); /* In case there is no value to convert. */ if(p->change==NULL) return; /* Do the conversion on all channels for each change. */ for(change=p->change; change!=NULL; change=change->next) for(channel=p->chll; channel!=NULL; channel=channel->next) { /* Make a condition array: all pixels with a value equal to `change->from' will be set as 1 in this array. */ cond=gal_arithmetic(GAL_ARITHMETIC_OP_EQ, GAL_ARITHMETIC_NUMOK, channel, change->from); /* Now, use the condition array to set the proper values. */ channel=gal_arithmetic(GAL_ARITHMETIC_OP_WHERE, flags, channel, cond, change->to); /* Clean up, since we set the free flag, all extra arrays have been freed.*/ gal_data_free(change->from); } /* Free the channels linked list. */ change=p->change; while(change!=NULL) { tmp=change->next; free(change); change=tmp; } } static void convertt_trunc_function(int operator, gal_data_t *data, gal_data_t *value) { gal_data_t *cond, *out; /* Note that we need the fluxlow and fluxhigh values later. */ unsigned char flags = ( GAL_ARITHMETIC_NUMOK | GAL_ARITHMETIC_INPLACE ); /* Make a condition array: all pixels with a value equal to `change->from' will be set as 1 in this array. */ cond=gal_arithmetic(operator, GAL_ARITHMETIC_NUMOK, data, value); /* Now, use the condition array to set the proper values. */ out=gal_arithmetic(GAL_ARITHMETIC_OP_WHERE, flags, data, cond, value); /* A small sanity check. The process must be in-place so the original data structure must not have changed. */ if(out!=data) error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to solve the " "problem. The `out' and `data' pointers are the same", __func__, PACKAGE_BUGREPORT); /* Clean up. */ gal_data_free(cond); } static void convertt_truncate(struct converttparams *p) { gal_data_t *channel; /* Return if no truncation is desired. */ if(p->fluxhigh==NULL && p->fluxlow==NULL) return; /* Do the truncation for each channel. */ for(channel=p->chll; channel!=NULL; channel=channel->next) { if(p->fluxlow) convertt_trunc_function(GAL_ARITHMETIC_OP_LT, channel, p->fluxlow); if(p->fluxhigh) convertt_trunc_function(GAL_ARITHMETIC_OP_GT, channel, p->fluxhigh); } } /**************************************************************/ /************** Save text and FITS ***************/ /**************************************************************/ static void save_with_gnuastro_lib(struct converttparams *p) { gal_data_t *channel; /* Determine the type. */ switch(p->outformat) { /* FITS: a FITS file can have many extensions (channels). */ case OUT_FORMAT_FITS: for(channel=p->chll; channel!=NULL; channel=channel->next) gal_fits_img_write(channel, p->cp.output, NULL, PROGRAM_NAME); break; /* Plain text: only one channel is acceptable. */ case OUT_FORMAT_TXT: gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); gal_txt_write(p->chll, NULL, p->cp.output); break; /* Not recognized. */ default: error(EXIT_FAILURE, 0, "%s: a bug! output format code `%d' not " "recognized", __func__, p->outformat); } } /**************************************************************/ /************** convert to 8 bit ***************/ /**************************************************************/ void convertt_scale_to_uchar(struct converttparams *p) { size_t size=p->chll->size; unsigned char *u, *fu, maxbyte=p->maxbyte; gal_data_t *channel, *prev, *copied, *mind, *maxd; float *f, *ff, m, tmin, tmax, min=FLT_MAX, max=-FLT_MAX; /* Convert everything to single precision floating point type and find the minimum and maximum values of all the channels in the process. */ prev=NULL; for(channel=p->chll; channel!=NULL; channel=channel->next) { /* Only for channels that weren't originally blank. */ if(channel->status==0) { /* If the type isn't float, then convert it to float. */ if(channel->type!=GAL_TYPE_FLOAT32) { /* Change the type to float. */ copied=gal_data_copy_to_new_type(channel, GAL_TYPE_FLOAT32); /* Correct the pointers. */ copied->next=channel->next; if(prev) prev->next=copied; else p->chll=copied; /* Clean the old data structure and put in the new one */ gal_data_free(channel); channel=copied; } /* Calculate the minimum and maximum. */ mind = gal_arithmetic(GAL_ARITHMETIC_OP_MINVAL, 0, channel); maxd = gal_arithmetic(GAL_ARITHMETIC_OP_MAXVAL, 0, channel); tmin = *((float *)(mind->array)); tmax = *((float *)(maxd->array)); gal_data_free(mind); gal_data_free(maxd); /* See the over-all minimum and maximum values. */ if(tmin<min) min=tmin; if(tmax>max) max=tmax; } /* Set the prev pointer. */ prev=channel; } /* Change the minimum and maximum if desired, Note that this is only non-redundant when fluxhigh and fluxlow are more or less than the maximum and minimum values in the image.*/ if(p->fluxlow || p->fluxhigh) { if(p->flminbyte) { /* Convert the fluxlow value to float and put it in min. */ copied=gal_data_copy_to_new_type(p->fluxlow, GAL_TYPE_FLOAT32); min = *((float *)(copied->array)); gal_data_free(copied); } if(p->fhmaxbyte) { /* Convert the fluxhigh value to float and put it in min. */ copied=gal_data_copy_to_new_type(p->fluxhigh, GAL_TYPE_FLOAT32); max = *((float *)(copied->array)); gal_data_free(copied); } } m=(float)maxbyte/(max-min); /* Convert all the non-blank channels to unsigned char. */ prev=NULL; for(channel=p->chll; channel!=NULL; channel=channel->next) { if(channel->status==0) { /* Convert the values into a range between `0' and `maxbyte'. */ ff=(f=channel->array)+size; if(p->invert) { do *f = isnan(*f) ? maxbyte : maxbyte-(*f-min)*m; while(++f<ff); } else { do *f = isnan(*f) ? 0 : (*f-min)*m; while(++f<ff); } /* Change the type to unsigned char. */ copied=gal_data_copy_to_new_type(channel, GAL_TYPE_UINT8); /* Correct the pointers. */ copied->next=channel->next; if(prev) prev->next=copied; else p->chll=copied; /* Clean the old data structure and put in the new one */ gal_data_free(channel); channel=copied; } else { /* In CMYK, a blank channel should have a maximum value. */ if(p->numch==4) {fu=(u=channel->array)+size; do *u=UINT8_MAX; while(++u<fu);} } /* Set the prev pointer. */ prev=channel; } } /**************************************************************/ /************** Main function ***************/ /**************************************************************/ void convertt(struct converttparams *p) { /* Make any of the desired changes to the data. */ if(p->changeaftertrunc) { convertt_truncate(p); convertt_change(p); } else { convertt_change(p); convertt_truncate(p); } /* Save the outputs: */ switch(p->outformat) { case OUT_FORMAT_TXT: case OUT_FORMAT_FITS: save_with_gnuastro_lib(p); break; case OUT_FORMAT_JPEG: #ifdef HAVE_LIBJPEG convertt_scale_to_uchar(p); jpeg_write(p); #else error(EXIT_FAILURE, 0, "you have asked for a JPEG output, however, " "when %s was configured libjpeg was not available. To write " "to JPEG files, libjpeg is required. Please install it and " "configure, make and install %s again", PACKAGE_STRING, PACKAGE_STRING); #endif break; case OUT_FORMAT_EPS: case OUT_FORMAT_PDF: convertt_scale_to_uchar(p); eps_write_eps_or_pdf(p); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us so we can find " "the problem and fix it The internal type of the output is " "not recognized. ", __func__); } } ��������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/ui.c����������������������������������������������������������������������0000644�0001750�0001750�00000056730�13174462540�013357� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2016, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/txt.h> #include <gnuastro/wcs.h> #include <gnuastro/list.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro/blank.h> #include <gnuastro/arithmetic.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "eps.h" #include "jpeg.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "InputFile1 [InputFile2] ... [InputFile4]"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will convert any of the " "known input formats to any other of the known formats. The output file " "will have the same number of pixels.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct converttparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* Program specific non-zero values. */ p->maxbyte = UINT8_MAX; p->quality = GAL_BLANK_UINT8; /* Modify the common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: cp->coptions[i].value=&p->hdus; cp->coptions[i].type=GAL_TYPE_STRLL; cp->coptions[i].doc="FITS input HDU, multiple calls possible."; break; case GAL_OPTIONS_KEY_OUTPUT: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; cp->coptions[i].doc="Output filename or suffix."; break; case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct converttparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: gal_list_str_add(&p->inputnames, arg, 0); break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct converttparams *p) { gal_data_t *cond; /* Read the truncation values into a data structure and see if flux low is indeed smaller than fluxhigh. */ if(p->fluxlowstr) { p->fluxlow=gal_data_copy_string_to_number(p->fluxlowstr); if(p->fluxlow==NULL) error(EXIT_FAILURE, 0, "value to the `--fluxlow' (`-L', %s) " "couldn't be read as a number", p->fluxlowstr); } if(p->fluxhighstr) { p->fluxhigh=gal_data_copy_string_to_number(p->fluxhighstr); if(p->fluxhigh==NULL) error(EXIT_FAILURE, 0, "value to the `--fluxhigh' (`-H', %s) " "couldn't be read as a number", p->fluxhighstr); } if(p->fluxhighstr && p->fluxlowstr) { cond=gal_arithmetic(GAL_ARITHMETIC_OP_GT, GAL_ARITHMETIC_NUMOK, p->fluxhigh, p->fluxlow); if( *((unsigned char *)cond->array) == 0 ) error(EXIT_FAILURE, 0, "The value of `--fluxlow' must be less " "than `--fluxhigh'"); gal_data_free(cond); } } static void ui_check_options_and_arguments(struct converttparams *p) { /* Check if there was any inputs. */ if(p->inputnames==NULL) error(EXIT_FAILURE, 0, "no input files given"); /* Reverse the `inputnames' linked list, note that the `hdu' linked list was reversed during option parsing.*/ gal_list_str_reverse(&p->inputnames); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ static struct change * ui_make_change_struct(char *arg) { char *p=arg; gal_data_t *data; size_t len=0, counter=0; struct change *out=NULL, *last=NULL, *ch; /* First set all the delimiters to `\0' and count the number of characters in the full string. */ while(*p!='\0') { if( isspace(*p) || *p==':' || *p==',' ) *p='\0'; ++p; } len=p-arg; /* Now, go through the string and read everything that remains. */ p=arg; while(p<arg+len) { if(*p=='\0') ++p; else { /* Read the number and increment the counter. */ ++counter; data=gal_data_copy_string_to_number(p); if(data==NULL) error(EXIT_FAILURE, 0, "`%s' (input number %zu to the " "`--change' option) couldn't be read as a number", p, counter); /* Go to the end of this number (until you reach a `\0'). */ while(*p!='\0') {++p; continue;} /* Put the data structure in the correct place. When the counter is an odd number, we have just started a new set of changes.*/ if(counter%2) /* Odd. */ { /* Allocate space for the new structure. */ errno=0; ch=malloc(sizeof *ch); if(ch==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `ch'", __func__, sizeof *ch); /* If the last structure has already been defined (!=NULL) then we should set its next element to `ch' and change it to point to `ch'. On the other hand, when this is the first structure to be created, then `last==NULL', so to start off the process, we should put `ch' into both the `out' and `last' lists.. */ if(last) { last->next=ch; last=ch; } else out=last=ch; /* Put `data' in the `from' element, and since this is the last structure, set its next element to NULL. */ last->from=data; last->next=NULL; } else /* Even. */ last->to=data; } } /* { struct change *tmp; for(tmp=out;tmp!=NULL;tmp=tmp->next) printf("%f --> %f\n", tmp->from, tmp->to); } */ return out; } /* Go through the input files and make a linked list of all the channels that exist in them. When this function finishes the list of channels will be filled in the same order as they were read from the inputs. */ static void ui_make_channels_ll(struct converttparams *p) { char *hdu=NULL; size_t dsize=0; gal_data_t *data; gal_list_str_t *name; /* Go through the input files and add the channel(s). */ p->numch=0; for(name=p->inputnames; name!=NULL; name=name->next) { /* Check if p->numch has not exceeded 4. */ if(p->numch>=4) error(EXIT_FAILURE, 0, "the number of input color channels (not " "necessarily files) has exceeded 4! Note that one file can " "contain more than one color channel (for example a JPEG " "file in RGB has 3 channels)"); /* Make sure this input file exists (if it isn't blank). */ if(strcmp(name->v, "blank")) gal_checkset_check_file(name->v); /* FITS: */ if( gal_fits_name_is_fits(name->v) ) { /* Get the HDU value for this channel. */ if(p->hdus) hdu=gal_list_str_pop(&p->hdus); else error(EXIT_FAILURE, 0, "not enough HDUs. Every input FITS image " "needs a HDU, you can use the `--hdu' (`-h') option once " "for each input FITS image (in the same order)"); /* Read in the array and its WCS information. */ data=gal_fits_img_read(name->v, hdu, p->cp.minmapsize, 0, 0); gal_list_data_add(&p->chll, data); /* A FITS file only has one channel. */ ++p->numch; } /* JPEG: */ else if ( nameisjpeg(name->v) ) { #ifndef HAVE_LIBJPEG error(EXIT_FAILURE, 0, "you are giving a JPEG input, however, " "when %s was configured libjpeg was not available. To read " "from (and write to) JPEG files, libjpeg is required. " "Please install it and configure, make and install %s " "again", PACKAGE_STRING, PACKAGE_STRING); #else p->numch += jpeg_read_to_ll(name->v, &p->chll, p->cp.minmapsize); #endif } /* Blank: */ else if(strcmp(name->v, BLANK_CHANNEL_NAME)==0) { gal_list_data_add_alloc(&p->chll, NULL, GAL_TYPE_INVALID, 0, &dsize, NULL, 0, p->cp.minmapsize, "blank", NULL, NULL); ++p->numch; } /* EPS: */ else if ( nameiseps(name->v) ) error(EXIT_FAILURE, 0, "EPS files cannot be used as input. Since " "EPS files are not raster graphics, they are only used as " "output"); /* PDF: */ else if ( nameispdf(name->v) ) error(EXIT_FAILURE, 0, "PDF files cannot be used as input. Since " "PDF files are not raster graphics, they are only used as " "output"); /* Text: */ else { data=gal_txt_image_read(name->v, p->cp.minmapsize); gal_list_data_add(&p->chll, data); ++p->numch; } } /* Reverse the list of channels into the input order. */ gal_list_data_reverse(&p->chll); } /* Read the input(s)/channels. */ static void ui_prepare_input_channels(struct converttparams *p) { struct wcsprm *wcs=NULL; size_t i, ndim=0, *dsize=NULL; gal_data_t *tmp, *blank, *prev; /* Fill in the channels linked list. */ ui_make_channels_ll(p); /* Make sure there are 1 (for grayscale), 3 (for RGB) or 4 (for CMYK) color channels. */ if(p->numch!=1 && p->numch!=3 && p->numch!=4) error(EXIT_FAILURE, 0, "the number of input color channels has to be " "1 (for non image data, grayscale or only K channel in CMYK), " "3 (for RGB) and 4 (for CMYK). You have given %zu color channels. " "Note that some file formats (for example JPEG in RGB mode) can " "contain more than one color channel", p->numch); /* Go over the channels and make the proper checks/corrections. We won't be checking blank channels here, recall that blank channels had a dimension of zero. */ for(tmp=p->chll; tmp!=NULL; tmp=tmp->next) if(tmp->ndim>0) { /* Set the reference size (to check and also use for the blank channels). */ if(dsize==NULL) { ndim=tmp->ndim; dsize=tmp->dsize; } else { if(tmp->ndim!=ndim) error(EXIT_FAILURE, 0, "All channels must have the same " "number of dimensions, the first input channel had " "%zu dimensions while atleast one other has %zu", ndim, tmp->ndim); for(i=0;i<ndim;++i) if(dsize[i]!=tmp->dsize[i]) error(EXIT_FAILURE, 0, "The length along each dimension of " "the channels must be the same"); } /* Incase there is WCS information, also keep a pointer to the first WCS information encountered. */ if(wcs==NULL && tmp->wcs) wcs=tmp->wcs; } /* If ndim is still NULL, then there were no non-blank inputs, so print an error. */ if(dsize==NULL) error(EXIT_FAILURE, 0, "all the input(s) are of type blank"); /* Now, fill in the blank channels with zero valued arrays. */ prev=NULL; for(tmp=p->chll; tmp!=NULL; tmp=tmp->next) { /* If this is a blank structure, then set it to a zero valued array. */ if(tmp->ndim==0) { /* Make the blank data structure. */ blank=gal_data_alloc(NULL, GAL_TYPE_UINT8, ndim, dsize, wcs, 1, p->cp.minmapsize, "blank channel", NULL, NULL); /* We will use the status value of the data structuer to mark it as one that was originally blank. */ blank->status=1; /* If a previous node pointed to this old blank structure, then correct it. */ if(prev) prev->next=blank; else p->chll=blank; /* Set the next pointer of this one to same pointer that the old blank pointer pointed to. */ blank->next=tmp->next; /* Free the old data structure and put this one in its place. */ gal_data_free(tmp); tmp=blank; } /* This is the final (to be used) data structure, so keep its pointer in case the next one is blank and this structure's `next' element must be corrected. */ prev=tmp; } } /* We know cp->output is a known suffix, we just don't know if it has a `.` before it or not. If it doesn't, one will be added to it and the output name will be set using the automatic output function. */ void ui_add_dot_use_automatic_output(struct converttparams *p) { gal_list_str_t *stll; char *tmp, *firstname="output.txt", *suffix=p->cp.output; /* Find the first non-blank file name in the input(s). */ for(stll=p->inputnames; stll!=NULL; stll=stll->next) if(strcmp(stll->v, BLANK_CHANNEL_NAME)) { firstname=stll->v; break; } /* If the suffix does not start with a `.', put one there. */ if(suffix[0]!='.') { asprintf(&tmp, ".%s", suffix); free(suffix); suffix=tmp; } /* Set the automatic output and make sure we have write access. */ p->cp.output=gal_checkset_automatic_output(&p->cp, firstname, suffix); } /* Set output name, not that for ConvertType, the output option value is mandatory (in `args.h'). So by the time the program reaches here, we know it exists. */ static void ui_set_output(struct converttparams *p) { struct gal_options_common_params *cp=&p->cp; /* Determine the type */ if(gal_fits_name_is_fits(cp->output)) { p->outformat=OUT_FORMAT_FITS; if( gal_fits_suffix_is_fits(cp->output) ) ui_add_dot_use_automatic_output(p); } else if(nameisjpeg(cp->output)) { #ifndef HAVE_LIBJPEG error(EXIT_FAILURE, 0, "you have asked for a JPEG output, " "however, when %s was configured libjpeg was not " "available. To write to JPEG files, libjpeg is required. " "Please install it and configure, make and install %s " "again", PACKAGE_STRING, PACKAGE_STRING); #else /* Small sanity checks. */ if(p->quality == GAL_BLANK_UINT8) error(EXIT_FAILURE, 0, "the `--quality' (`-u') option is necessary for " "jpeg outputs, but it has not been given"); if(p->quality > 100) error(EXIT_FAILURE, 0, "`%u' is larger than 100. The value to the " "`--quality' (`-u') option must be between 1 and 100 (inclusive)", p->quality); /* Preparations. */ p->outformat=OUT_FORMAT_JPEG; if( nameisjpegsuffix(cp->output) ) ui_add_dot_use_automatic_output(p); #endif } else if(nameiseps(cp->output)) { p->outformat=OUT_FORMAT_EPS; if( nameisepssuffix(cp->output) ) ui_add_dot_use_automatic_output(p); } else if(nameispdf(cp->output)) { p->outformat=OUT_FORMAT_PDF; if( nameispdfsuffix(cp->output) ) ui_add_dot_use_automatic_output(p); } else { p->outformat=OUT_FORMAT_TXT; /* If the given value is `stdout', then set p->cp.output to NULL, so the result will be printed to the standard output. */ if( !strcmp(p->cp.output, "stdout") ) { free(p->cp.output); p->cp.output=NULL; } else { /* Plain text files don't have any unique set of suffixes. So, here, we will just adopt two of the most common ones: `txt' or `dat'. If the output is just one of these two suffixes, then we will use automatic output to generate the full name, otherwise, we'll just take the user's given value as the filename. */ if( !strcmp(cp->output, "txt") || !strcmp(cp->output, ".txt") || !strcmp(cp->output, "dat") || !strcmp(cp->output, ".dat") ) ui_add_dot_use_automatic_output(p); /* If output type is not an image, there should only be one color channel: */ if(p->numch>1) error(EXIT_FAILURE, 0, "text output (`--output=%s`) can only be " "completed with one input color channel. You have given " "%zu. Note that some formats (for example JPEG) can have " "more than one color channel in each file. You can first " "convert the file to FITS, then convert the desired " "channel to text by specifying the HDU", cp->output, p->numch); } } /* Check if the output already exists. */ gal_checkset_writable_remove(cp->output, 0, cp->dontdelete); } void ui_preparations(struct converttparams *p) { /* Convert the change string into the proper list. */ if(p->changestr) p->change=ui_make_change_struct(p->changestr); /* Read the input channels. */ ui_prepare_input_channels(p); /* Set the output name. */ ui_set_output(p); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct converttparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct converttparams *p) { /* Free the allocated spaces */ gal_data_free(p->fluxlow); gal_data_free(p->fluxhigh); gal_list_str_free(p->hdus, 1); if(p->cp.output) free(p->cp.output); gal_list_str_free(p->inputnames, 0); } ����������������������������������������gnuastro-0.5/bin/convertt/main.c��������������������������������������������������������������������0000644�0001750�0001750�00000003044�13121462410�013640� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* ConvertType - Convert between various types of files. ConvertType is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" /* needs main.h. */ #include "convertt.h" int main(int argc, char *argv[]) { struct converttparams p={{{0},0},0}; /* Set the starting time.*/ time(&p.rawtime); /* Read the input parameters.*/ ui_read_check_inputs_setup(argc, argv, &p); /* Run Convert. */ convertt(&p); /* Free all non-freed allocations. */ ui_free_report(&p); /* Return successfully.*/ return EXIT_SUCCESS; } 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= @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @SYS_IOCTL_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ SYS_TIME_H_DEFINES_STRUCT_TIMESPEC = @SYS_TIME_H_DEFINES_STRUCT_TIMESPEC@ TIME_H_DEFINES_STRUCT_TIMESPEC = @TIME_H_DEFINES_STRUCT_TIMESPEC@ UINT32_MAX_LT_UINTMAX_MAX = @UINT32_MAX_LT_UINTMAX_MAX@ UINT64_MAX_EQ_ULONG_MAX = @UINT64_MAX_EQ_ULONG_MAX@ UNDEFINE_STRTOK_R = @UNDEFINE_STRTOK_R@ UNISTD_H_DEFINES_STRUCT_TIMESPEC = @UNISTD_H_DEFINES_STRUCT_TIMESPEC@ UNISTD_H_HAVE_WINSOCK2_H = @UNISTD_H_HAVE_WINSOCK2_H@ UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS = @UNISTD_H_HAVE_WINSOCK2_H_AND_USE_SOCKETS@ VERSION = @VERSION@ WCHAR_T_SUFFIX = @WCHAR_T_SUFFIX@ WINDOWS_64_BIT_OFF_T = @WINDOWS_64_BIT_OFF_T@ WINDOWS_64_BIT_ST_SIZE = @WINDOWS_64_BIT_ST_SIZE@ WINDOWS_STAT_INODES = @WINDOWS_STAT_INODES@ WINDOWS_STAT_TIMESPEC = @WINDOWS_STAT_TIMESPEC@ WINT_T_SUFFIX = @WINT_T_SUFFIX@ YIELD_LIB = @YIELD_LIB@ abs_builddir = @abs_builddir@ abs_srcdir = @abs_srcdir@ abs_top_builddir = @abs_top_builddir@ abs_top_srcdir = @abs_top_srcdir@ ac_ct_AR = @ac_ct_AR@ ac_ct_CC = @ac_ct_CC@ ac_ct_CXX = @ac_ct_CXX@ ac_ct_DUMPBIN = @ac_ct_DUMPBIN@ am__include = @am__include@ am__leading_dot = @am__leading_dot@ am__quote = @am__quote@ am__tar = @am__tar@ am__untar = @am__untar@ ax_pthread_config = @ax_pthread_config@ bindir = @bindir@ build = @build@ build_alias = @build_alias@ build_cpu = @build_cpu@ build_os = @build_os@ build_vendor = @build_vendor@ builddir = @builddir@ datadir = @datadir@ datarootdir = @datarootdir@ docdir = @docdir@ dvidir = @dvidir@ exec_prefix = @exec_prefix@ gl_LIBOBJS = @gl_LIBOBJS@ gl_LTLIBOBJS = @gl_LTLIBOBJS@ gltests_LIBOBJS = @gltests_LIBOBJS@ gltests_LTLIBOBJS = @gltests_LTLIBOBJS@ gltests_WITNESS = @gltests_WITNESS@ has_ghostscript = @has_ghostscript@ has_glibtool = @has_glibtool@ has_help2man = @has_help2man@ has_libtool = @has_libtool@ host = @host@ host_alias = @host_alias@ host_cpu = @host_cpu@ host_os = @host_os@ host_vendor = @host_vendor@ htmldir = @htmldir@ includedir = 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for ConvertType. # ConvertType is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. 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This file is offered as-is, without any # warranty. # Input: # Output: quality 100 widthincm 10.0 borderwidth 1 output jpg # Flux: invert 0 # Common options ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/convertt/Makefile.am���������������������������������������������������������������0000644�0001750�0001750�00000002634�13121462410�014610� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astconvertt astconvertt_LDADD = -lgnuastro astconvertt_SOURCES = main.c ui.c convertt.c eps.c jpeg.c EXTRA_DIST = main.h authors-cite.h args.h ui.h convertt.h eps.h jpeg.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astconvertt.conf ����������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/�������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�012763� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/buildprog.h��������������������������������������������������������������0000644�0001750�0001750�00000002115�13121462410�015031� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef BUILDPROG_H #define BUILDPROG_H int buildprog(struct buildprogparams *p); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/ui.h���������������������������������������������������������������������0000644�0001750�0001750�00000003440�13211076737�013476� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Available letters for short options: c d e f i j k n p r s t u v w x y z A B C E G H J Q R X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_INCLUDE = 'I', UI_KEY_LINKDIR = 'L', UI_KEY_LINKLIB = 'l', UI_KEY_LA = 'a', UI_KEY_ONLYBUILD = 'b', UI_KEY_DEBUG = 'g', UI_KEY_OPTIMIZE = 'O', UI_KEY_WARNING = 'W', /* Only with long version (start with a value 1000, the rest will be set automatically). */ UI_KEY_DETELECOMPILED = 1000, UI_KEY_TAG, }; void ui_read_check_inputs_setup(int argc, char *argv[], struct buildprogparams *p); void ui_free_report(struct buildprogparams *p); #endif ��������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/args.h�������������������������������������������������������������������0000644�0001750�0001750�00000010775�13211076737�014026� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Array of acceptable options. */ struct argp_option program_options[] = { { "includedir", UI_KEY_INCLUDE, "STR", 0, "Directories to search for `#include's.", GAL_OPTIONS_GROUP_INPUT, &p->include, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "linkdir", UI_KEY_LINKDIR, "STR", 0, "Directory to search for libraries to link.", GAL_OPTIONS_GROUP_INPUT, &p->linkdir, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "linklib", UI_KEY_LINKLIB, "STR", 0, "Link libraries, e.g., for libgsl: `-lgsl'.", GAL_OPTIONS_GROUP_INPUT, &p->linklib, GAL_TYPE_STRLL, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "la", UI_KEY_LA, "STR", 0, "Libtool `.la' to use instead of default.", GAL_OPTIONS_GROUP_INPUT, &p->la, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "tag", UI_KEY_TAG, "STR", 0, "Libtool `--tag': programming language.", GAL_OPTIONS_GROUP_INPUT, &p->tag, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "debug", UI_KEY_DEBUG, 0, 0, "Debugging information in compiled binary.", GAL_OPTIONS_GROUP_OUTPUT, &p->debug, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "optimize", UI_KEY_OPTIMIZE, "INT", 0, "Optimization level: 0, 1, 2, 3.", GAL_OPTIONS_GROUP_OUTPUT, &p->optimize, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "warning", UI_KEY_WARNING, "STR", 0, "Compilation warnings on command-line.", GAL_OPTIONS_GROUP_OUTPUT, &p->warning, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "onlybuild", UI_KEY_ONLYBUILD, 0, 0, "Don't run the built program.", GAL_OPTIONS_GROUP_OUTPUT, &p->onlybuild, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_0_OR_1, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, { "deletecompiled", UI_KEY_DETELECOMPILED, 0, 0, "Delete compiled program after running.", GAL_OPTIONS_GROUP_OUTPUT, &p->deletecompiled, GAL_OPTIONS_NO_ARG_TYPE, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure ------------------------------- NOTE: these parts can be left untouched.*/ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ���gnuastro-0.5/bin/buildprog/authors-cite.h�����������������������������������������������������������0000644�0001750�0001750�00000003011�13211076737�015462� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/main.h�������������������������������������������������������������������0000644�0001750�0001750�00000004667�13211076737�014021� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H /* Include necessary headers */ #include <gnuastro/data.h> #include <gnuastro-internal/options.h> /* Progarm names. */ #define PROGRAM_NAME "BuildProgram" /* Program full name. */ #define PROGRAM_EXEC "astbuildprog" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Main program parameters structure */ struct buildprogparams { /* From command-line */ struct gal_options_common_params cp; /* Common parameters. */ gal_list_str_t *sourceargs; /* Source files and arguments. */ gal_list_str_t *include; /* Libraries to link against. */ gal_list_str_t *linkdir; /* Libraries to link against. */ gal_list_str_t *linklib; /* Libraries to link against. */ char *la; /* Libtool `.la' instead of default. */ char *tag; /* Libtool tag (programming language).*/ char *optimize; /* Optimization level. */ char *debug; /* Keep debugging information. */ char *warning; /* Compiler warnings. */ uint8_t onlybuild; /* Don't run the compiled program. */ uint8_t deletecompiled; /* Delete compiled program after running. */ /* Output: */ time_t rawtime; /* Starting time of the program. */ }; #endif �������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/buildprog.c��������������������������������������������������������������0000644�0001750�0001750�00000011627�13211076737�015051� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <stdlib.h> #include <string.h> #include <gnuastro/list.h> #include <main.h> /* Write the given list into */ char * buildprog_as_one_string(char *opt, gal_list_str_t *list) { char *out; size_t len=0; gal_list_str_t *tmp; /* Only if we have a list. */ if(list) { /* For every node in the list, we want the `opt' and a space along with the actual string. */ for(tmp=list; tmp!=NULL; tmp=tmp->next) len += 1 + (opt ? strlen(opt) : 0) + strlen(tmp->v); /* Allocate space for the string. */ out=gal_data_malloc_array(GAL_TYPE_UINT8, len+1, __func__, "out"); /* Write all the strings into the allocated space. */ len=0; for(tmp=list; tmp!=NULL; tmp=tmp->next) len += sprintf(&out[len], "%s%s ", opt ? opt : "", tmp->v); } else out=NULL; /* Return the final string. */ return out; } int buildprog(struct buildprogparams *p) { /* Note that the first node of `sourceargs' is the acutal source and the rest are arguments to be run later. */ int retval; char *fullla; char *command, *optimize=NULL, *warning=NULL; char *include = buildprog_as_one_string("-I", p->include); char *linkdir = buildprog_as_one_string("-L", p->linkdir); char *linklib = buildprog_as_one_string("-l", p->linklib); char *arguments = buildprog_as_one_string(NULL, p->sourceargs->next); /* If not in quiet mode, let the user know. */ if(!p->cp.quiet) { printf("\nCompiling and linking the program\n"); printf("---------------------------------\n"); } /* Compiler options with values: */ if(p->warning) asprintf(&warning, "-W%s", p->warning); if(p->optimize) asprintf(&optimize, "-O%s", p->optimize); /* Libtool `.la' file: */ if(p->la) fullla=p->la; else asprintf(&fullla, "%s/libgnuastro.la", LIBDIR); /* Put the command to run into a string. */ asprintf(&command, "%s %s %s%s --mode=link gcc %s %s %s %s %s %s %s " "-I%s %s -o %s", GAL_CONFIG_GNULIBTOOL_EXEC, p->cp.quiet ? "--quiet" : "", p->tag ? "--tag=" : "", p->tag ? p->tag : "", warning ? warning : "", p->debug ? "-g" : "", optimize ? optimize : "", include ? include : "", linkdir ? linkdir : "", p->sourceargs->v, linklib ?linklib : "", INCLUDEDIR, fullla, p->cp.output); /* Compile (and link): */ retval=system(command); if(retval!=EXIT_SUCCESS) error(EXIT_FAILURE, 0, "failed to build, see libtool error above"); else if(p->onlybuild==0) { /* Free the initial command. */ free(command); /* Wright the command to run the program. Note that if the output value doesn't start with a directory, we'll have to put one for it. */ switch(p->cp.output[0]) { case '.': case '/': asprintf(&command, "%s %s", p->cp.output, arguments?arguments:""); break; default: asprintf(&command, "./%s %s", p->cp.output, arguments?arguments:""); } /* Print the executed command if necessary, then run it. */ if(!p->cp.quiet) { printf("\nRun the compiled program\n"); printf("------------------------\n"); printf("%s\n", command); } retval=system(command); /* Delete the compiled program after running it. */ if(p->deletecompiled) { errno=0; if( remove(p->cp.output) == -1 ) error(EXIT_FAILURE, 0, "unable to delete %s", p->cp.output); } } /* Clean up and return. */ free(include); free(linkdir); free(linklib); free(command); if(warning) free(warning); if(optimize) free(optimize); if(!p->la && fullla) free(fullla); return retval; } ���������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/ui.c���������������������������������������������������������������������0000644�0001750�0001750�00000023515�13175442274�013500� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <string.h> #include <gnuastro/fits.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the Argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "C-source [ARGUMENTS TO RUN]"; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will compile and run a " "C program, while automatically linking with libraries that Gnuastro " "depends on. Hence you do not have to worry about explicitly linking " "with CFITSIO for example if you want to work on a FITS file, or with " "GSL if you want to use GNU Scientific Library's functions. The standard " "compiler options of `-I', `-L', and `-l' are also available for further " "customization of the build.\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct buildprogparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* Modify common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_LOG: case GAL_OPTIONS_KEY_HDU: case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_NUMTHREADS: case GAL_OPTIONS_KEY_MINMAPSIZE: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; cp->coptions[i].mandatory=GAL_OPTIONS_NOT_MANDATORY; break; /* `--ignorecase's default short format is `I', but here we want to follow the compiler format, hence we need `I' for `include'. Therefore, here, we'll change the key for `include' to some large number just to avoid confusion.*/ case GAL_OPTIONS_KEY_IGNORECASE: cp->coptions[i].key=20000; cp->coptions[i].flags=OPTION_HIDDEN; cp->coptions[i].mandatory=GAL_OPTIONS_NOT_MANDATORY; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct buildprogparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: gal_list_str_add(&p->sourceargs, arg, 0); break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Read and check ONLY the options. When arguments are involved, do the check in `ui_check_options_and_arguments'. */ static void ui_read_check_only_options(struct buildprogparams *p) { size_t len; /* If an `.la' file is given, make sure it has the correct suffix. */ if(p->la) { len=strlen(p->la); if(len>=4) if(strcmp(&p->la[len-3], ".la")) error(EXIT_FAILURE, 0, "`%s' is not a Libtool control file name " "(with a `.la' suffix). The file name given to the `--la' " "(`-a') option must be a Libtool control file", p->la); } } /* Check the options and arguments. */ static void ui_check_options_and_arguments(struct buildprogparams *p) { if(p->sourceargs==NULL) error(EXIT_FAILURE, 0, "no input (C source file) given"); } /**************************************************************/ /*************** Preparations *******************/ /**************************************************************/ void ui_preparations(struct buildprogparams *p) { /* Reverse the sourceargs list (note that the options are reversed in options.c). */ gal_list_str_reverse(&p->sourceargs); /* Set the final output name. `EXEEXT' comes from the configuration script (given by BuildProgram's `Makefile.am'). */ if(p->cp.output==NULL) p->cp.output=gal_checkset_automatic_output(&p->cp, p->sourceargs->v, EXEEXT); } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct buildprogparams *p) { struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files and set the common values. */ gal_options_read_config_set(&p->cp); /* Read the options into the program's structure, and check them and their relations prior to printing. */ ui_read_check_only_options(p); /* Print the option values if asked. Note that this needs to be done after the option checks so un-sane values are not printed in the output state. */ gal_options_print_state(&p->cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); /* Read/allocate all the necessary starting arrays. */ ui_preparations(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void ui_free_report(struct buildprogparams *p) { /* Free the allocated arrays: */ free(p->cp.hdu); free(p->cp.output); gal_list_str_free(p->include, 1); gal_list_str_free(p->linkdir, 1); gal_list_str_free(p->linklib, 1); gal_list_str_free(p->sourceargs, 0); } �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/buildprog/main.c�������������������������������������������������������������������0000644�0001750�0001750�00000003050�13121462410�013760� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* BuildProgram: Compile and run programs using Gnuastro's library BuildProgram is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" #include "buildprog.h" /* Main function */ int main (int argc, char *argv[]) { int retval; struct buildprogparams p={{{0},0},0}; /* Set they starting time. */ time(&p.rawtime); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ retval=buildprog(&p); /* Free all non-freed allocations. */ ui_free_report(&p); /* Return successfully.*/ return retval; } 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= @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = @REPLACE_LOGBF@ REPLACE_LOGBL = @REPLACE_LOGBL@ REPLACE_LOGF = @REPLACE_LOGF@ REPLACE_LOGL = @REPLACE_LOGL@ REPLACE_LSEEK = @REPLACE_LSEEK@ REPLACE_LSTAT = @REPLACE_LSTAT@ REPLACE_MALLOC = @REPLACE_MALLOC@ REPLACE_MBRLEN = @REPLACE_MBRLEN@ REPLACE_MBRTOWC = @REPLACE_MBRTOWC@ REPLACE_MBSINIT = @REPLACE_MBSINIT@ REPLACE_MBSNRTOWCS = @REPLACE_MBSNRTOWCS@ REPLACE_MBSRTOWCS = @REPLACE_MBSRTOWCS@ REPLACE_MBSTATE_T = @REPLACE_MBSTATE_T@ REPLACE_MBTOWC = @REPLACE_MBTOWC@ REPLACE_MEMCHR = @REPLACE_MEMCHR@ REPLACE_MEMMEM = @REPLACE_MEMMEM@ REPLACE_MKDIR = @REPLACE_MKDIR@ REPLACE_MKFIFO = @REPLACE_MKFIFO@ REPLACE_MKNOD = @REPLACE_MKNOD@ REPLACE_MKSTEMP = @REPLACE_MKSTEMP@ REPLACE_MKTIME = @REPLACE_MKTIME@ REPLACE_MODF = @REPLACE_MODF@ REPLACE_MODFF = @REPLACE_MODFF@ REPLACE_MODFL = @REPLACE_MODFL@ REPLACE_NAN = @REPLACE_NAN@ REPLACE_NANOSLEEP = @REPLACE_NANOSLEEP@ REPLACE_NL_LANGINFO = @REPLACE_NL_LANGINFO@ REPLACE_NULL = @REPLACE_NULL@ REPLACE_OBSTACK_PRINTF = @REPLACE_OBSTACK_PRINTF@ REPLACE_OPEN = @REPLACE_OPEN@ REPLACE_OPENAT = @REPLACE_OPENAT@ REPLACE_PERROR = @REPLACE_PERROR@ REPLACE_POPEN = @REPLACE_POPEN@ REPLACE_PREAD = @REPLACE_PREAD@ REPLACE_PRINTF = @REPLACE_PRINTF@ REPLACE_PSELECT = @REPLACE_PSELECT@ REPLACE_PTHREAD_SIGMASK = @REPLACE_PTHREAD_SIGMASK@ REPLACE_PTSNAME = @REPLACE_PTSNAME@ REPLACE_PTSNAME_R = @REPLACE_PTSNAME_R@ REPLACE_PUTENV = @REPLACE_PUTENV@ REPLACE_PWRITE = @REPLACE_PWRITE@ REPLACE_QSORT_R = @REPLACE_QSORT_R@ REPLACE_RAISE = @REPLACE_RAISE@ REPLACE_RANDOM_R = @REPLACE_RANDOM_R@ REPLACE_READ = @REPLACE_READ@ REPLACE_READLINK = @REPLACE_READLINK@ REPLACE_READLINKAT = @REPLACE_READLINKAT@ REPLACE_REALLOC = @REPLACE_REALLOC@ REPLACE_REALPATH = @REPLACE_REALPATH@ REPLACE_REMAINDER = @REPLACE_REMAINDER@ REPLACE_REMAINDERF = @REPLACE_REMAINDERF@ REPLACE_REMAINDERL = @REPLACE_REMAINDERL@ REPLACE_REMOVE = @REPLACE_REMOVE@ REPLACE_RENAME = @REPLACE_RENAME@ REPLACE_RENAMEAT = @REPLACE_RENAMEAT@ REPLACE_RMDIR = @REPLACE_RMDIR@ REPLACE_ROUND = @REPLACE_ROUND@ REPLACE_ROUNDF = @REPLACE_ROUNDF@ REPLACE_ROUNDL = @REPLACE_ROUNDL@ REPLACE_SELECT = @REPLACE_SELECT@ REPLACE_SETENV = @REPLACE_SETENV@ REPLACE_SETLOCALE = @REPLACE_SETLOCALE@ REPLACE_SIGNBIT = @REPLACE_SIGNBIT@ REPLACE_SIGNBIT_USING_GCC = @REPLACE_SIGNBIT_USING_GCC@ REPLACE_SINF = @REPLACE_SINF@ REPLACE_SINHF = @REPLACE_SINHF@ REPLACE_SLEEP = @REPLACE_SLEEP@ REPLACE_SNPRINTF = @REPLACE_SNPRINTF@ REPLACE_SPRINTF = @REPLACE_SPRINTF@ REPLACE_SQRTF = @REPLACE_SQRTF@ REPLACE_SQRTL = @REPLACE_SQRTL@ REPLACE_STAT = @REPLACE_STAT@ REPLACE_STDIO_READ_FUNCS = @REPLACE_STDIO_READ_FUNCS@ REPLACE_STDIO_WRITE_FUNCS = @REPLACE_STDIO_WRITE_FUNCS@ REPLACE_STPNCPY = @REPLACE_STPNCPY@ REPLACE_STRCASESTR = @REPLACE_STRCASESTR@ REPLACE_STRCHRNUL = @REPLACE_STRCHRNUL@ REPLACE_STRDUP = @REPLACE_STRDUP@ REPLACE_STRERROR = @REPLACE_STRERROR@ REPLACE_STRERROR_R = @REPLACE_STRERROR_R@ REPLACE_STRFTIME = @REPLACE_STRFTIME@ REPLACE_STRNCAT = @REPLACE_STRNCAT@ REPLACE_STRNDUP = @REPLACE_STRNDUP@ REPLACE_STRNLEN = @REPLACE_STRNLEN@ REPLACE_STRSIGNAL = @REPLACE_STRSIGNAL@ REPLACE_STRSTR = @REPLACE_STRSTR@ REPLACE_STRTOD = @REPLACE_STRTOD@ REPLACE_STRTOIMAX = @REPLACE_STRTOIMAX@ REPLACE_STRTOK_R = @REPLACE_STRTOK_R@ REPLACE_STRTOUMAX = @REPLACE_STRTOUMAX@ REPLACE_STRUCT_LCONV = @REPLACE_STRUCT_LCONV@ REPLACE_STRUCT_TIMEVAL = @REPLACE_STRUCT_TIMEVAL@ REPLACE_SYMLINK = @REPLACE_SYMLINK@ REPLACE_SYMLINKAT = @REPLACE_SYMLINKAT@ REPLACE_TANF = @REPLACE_TANF@ REPLACE_TANHF = @REPLACE_TANHF@ REPLACE_TIMEGM = @REPLACE_TIMEGM@ REPLACE_TMPFILE = @REPLACE_TMPFILE@ REPLACE_TOWLOWER = @REPLACE_TOWLOWER@ REPLACE_TRUNC = @REPLACE_TRUNC@ REPLACE_TRUNCATE = @REPLACE_TRUNCATE@ REPLACE_TRUNCF = @REPLACE_TRUNCF@ REPLACE_TRUNCL = @REPLACE_TRUNCL@ REPLACE_TTYNAME_R = @REPLACE_TTYNAME_R@ REPLACE_TZSET = @REPLACE_TZSET@ REPLACE_UNLINK = @REPLACE_UNLINK@ REPLACE_UNLINKAT = @REPLACE_UNLINKAT@ REPLACE_UNSETENV = @REPLACE_UNSETENV@ REPLACE_USLEEP = @REPLACE_USLEEP@ REPLACE_UTIMENSAT = @REPLACE_UTIMENSAT@ REPLACE_VASPRINTF = @REPLACE_VASPRINTF@ REPLACE_VDPRINTF = @REPLACE_VDPRINTF@ REPLACE_VFPRINTF = @REPLACE_VFPRINTF@ REPLACE_VPRINTF = @REPLACE_VPRINTF@ REPLACE_VSNPRINTF = @REPLACE_VSNPRINTF@ REPLACE_VSPRINTF = @REPLACE_VSPRINTF@ REPLACE_WCRTOMB = @REPLACE_WCRTOMB@ REPLACE_WCSFTIME = @REPLACE_WCSFTIME@ REPLACE_WCSNRTOMBS = @REPLACE_WCSNRTOMBS@ REPLACE_WCSRTOMBS = @REPLACE_WCSRTOMBS@ REPLACE_WCSWIDTH = @REPLACE_WCSWIDTH@ REPLACE_WCTOB = @REPLACE_WCTOB@ REPLACE_WCTOMB = @REPLACE_WCTOMB@ REPLACE_WCWIDTH = @REPLACE_WCWIDTH@ REPLACE_WRITE = @REPLACE_WRITE@ RESTRICT_REPLACEMENT = @RESTRICT_REPLACEMENT@ SED = @SED@ SET_MAKE = @SET_MAKE@ SHELL = @SHELL@ SIG_ATOMIC_T_SUFFIX = @SIG_ATOMIC_T_SUFFIX@ SIZEOF_LONG = @SIZEOF_LONG@ SIZEOF_SIZE_T = @SIZEOF_SIZE_T@ SIZE_T_SUFFIX = @SIZE_T_SUFFIX@ STDALIGN_H = @STDALIGN_H@ STDBOOL_H = @STDBOOL_H@ STDDEF_H = @STDDEF_H@ STDINT_H = @STDINT_H@ STRIP = @STRIP@ SYSEXITS_H = @SYSEXITS_H@ SYS_IOCTL_H_HAVE_WINSOCK2_H = @SYS_IOCTL_H_HAVE_WINSOCK2_H@ 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�����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for BuildProgram. # BuildProgram is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. 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This file is offered as-is, without any # warranty. # Output optimize 3 warning all tag CC ��������������������������������������������������������gnuastro-0.5/bin/buildprog/Makefile.am��������������������������������������������������������������0000644�0001750�0001750�00000003240�13164537456�014751� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Your Name <your@email> ## Contributing author(s): ## Copyright (C) YYYY, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. ## ## Buildprog will also need some system-specific information that is ## gathered at compile time (for example the library installation directory ## (LIBDIR) and the executive file suffix (EXEEXT). AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib -DLIBDIR=\"$(libdir)\" \ -DINCLUDEDIR=\"$(includedir)\" -DEXEEXT=\"$(EXEEXT)\" ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astbuildprog astbuildprog_LDADD = -lgnuastro astbuildprog_SOURCES = main.c ui.c buildprog.c EXTRA_DIST = main.h authors-cite.h args.h ui.h buildprog.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astbuildprog.conf ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/������������������������������������������������������������������������0000755�0001750�0001750�00000000000�13217220466�013125� 5����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/operands.h��������������������������������������������������������������0000644�0001750�0001750�00000002334�13121462410�015022� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef OPERANDS_H #define OPERANDS_H size_t operands_num(struct arithmeticparams *p); void operands_add(struct arithmeticparams *p, char *filename, gal_data_t *data); gal_data_t * operands_pop(struct arithmeticparams *p, char *operator); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/arithmetic.h������������������������������������������������������������0000644�0001750�0001750�00000002466�13173367042�015362� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef IMGARITH_H #define IMGARITH_H #include <gnuastro/arithmetic.h> /* These are operator codes for functions that aren't in the arithmetic library. */ enum arithmetic_prog_operators { ARITHMETIC_OP_FILTER_MEDIAN=GAL_ARITHMETIC_OP_LAST_CODE, ARITHMETIC_OP_FILTER_MEAN, }; void imgarith(struct arithmeticparams *p); #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/ui.h��������������������������������������������������������������������0000644�0001750�0001750�00000003051�13174462540�013635� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef UI_H #define UI_H /* For common options groups. */ #include <gnuastro-internal/options.h> /* Available letters for short options: a b c d e f i j k l m n p r s t u v w x y z A B C E G H J L O Q R W X Y */ enum option_keys_enum { /* With short-option version. */ UI_KEY_GLOBALHDU = 'g', /* Only with long version (start with a value 1000, the rest will be set automatically). */ }; void ui_read_check_inputs_setup(int argc, char *argv[], struct arithmeticparams *p); void freeandreport(struct arithmeticparams *p, struct timeval *t1); #endif ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/args.h������������������������������������������������������������������0000644�0001750�0001750�00000003652�13124332637�014161� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef ARGS_H #define ARGS_H /* Definition of program-specific options. */ struct argp_option program_options[] = { { "globalhdu", UI_KEY_GLOBALHDU, "STR", 0, "Use this HDU for all inputs, ignore `--hdu'.", GAL_OPTIONS_GROUP_INPUT, &p->globalhdu, GAL_TYPE_STRING, GAL_OPTIONS_RANGE_ANY, GAL_OPTIONS_NOT_MANDATORY, GAL_OPTIONS_NOT_SET }, {0} }; /* Define the child argp structure. */ struct argp gal_options_common_child = {gal_commonopts_options, gal_options_common_argp_parse, NULL, NULL, NULL, NULL, NULL}; /* Use the child argp structure in list of children (only one for now). */ struct argp_child children[]= { {&gal_options_common_child, 0, NULL, 0}, {0, 0, 0, 0} }; /* Set all the necessary argp parameters. */ struct argp thisargp = {program_options, parse_opt, args_doc, doc, children, NULL, NULL}; #endif ��������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/authors-cite.h����������������������������������������������������������0000644�0001750�0001750�00000002770�13211076737�015637� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2017, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef AUTHORS_CITE_H #define AUTHORS_CITE_H /* When any specific citation is necessary, please add its BibTeX (from ADS hopefully) to this variable along with a title decribing what this paper/book does for the progarm in a short line. In the following line put a row of `-' with the same length and then put the BibTeX. See the `gnuastro_bibtex' variable in `lib/options' (from the top Gnuastro source code directory) as an example.*/ #define PROGRAM_BIBTEX "" #define PROGRAM_AUTHORS "Mohammad Akhlaghi" #endif ��������gnuastro-0.5/bin/arithmetic/main.h������������������������������������������������������������������0000644�0001750�0001750�00000005334�13124332637�014150� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #ifndef MAIN_H #define MAIN_H #include <gnuastro/fits.h> #include <gnuastro/list.h> #include <gnuastro-internal/options.h> /* Progarm name macros: */ #define PROGRAM_NAME "Arithmetic" /* Program full name. */ #define PROGRAM_EXEC "astarithmetic" /* Program executable name. */ #define PROGRAM_STRING PROGRAM_NAME" (" PACKAGE_NAME ") " PACKAGE_VERSION /* Constants: */ #define NEG_DASH_REPLACE 11 /* Vertical tab (ASCII=11) for negative dash */ /* In every node of the operand linked list, only one of the `filename' or `data' should be non-NULL. Otherwise it will be a bug and will cause problems. All the operands operate on this premise. */ struct operand { char *filename; /* !=NULL if the operand is a filename. */ char *hdu; /* !=NULL if the operand is a filename. */ gal_data_t *data; /* !=NULL if the operand is a dataset. */ struct operand *next; /* Pointer to next operand. */ }; struct arithmeticparams { /* Other structures: */ struct gal_options_common_params cp; /* Common parameters. */ /* Input: */ gal_list_str_t *hdus; /* List of all given HDU strings. */ gal_list_str_t *tokens; /* List of all arithmetic tokens. */ size_t addcounter; /* The number of FITS images added. */ size_t popcounter; /* The number of FITS images popped. */ gal_data_t refdata; /* Container for information of the data. */ char *globalhdu; /* Single HDU for all inputs. */ /* Operating mode: */ /* Internal: */ struct operand *operands; /* The operands linked list. */ time_t rawtime; /* Starting time of the program. */ }; #endif ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/operands.c��������������������������������������������������������������0000644�0001750�0001750�00000012442�13164537456�015042� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "operands.h" size_t operands_num(struct arithmeticparams *p) { size_t counter=0; struct operand *tmp=NULL; for(tmp=p->operands;tmp!=NULL;tmp=tmp->next) ++counter; return counter; } void operands_add(struct arithmeticparams *p, char *filename, gal_data_t *data) { struct operand *newnode; /* Some operators might not actually return any dataset (data=NULL), in such cases filename will also be NULL (since the operand was not added from the command-line). So, we shouldn't add anything to the stack. */ if(data || filename) { /* Allocate space for the new operand. */ errno=0; newnode=malloc(sizeof *newnode); if(newnode==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for `newnode'", __func__, sizeof *newnode); /* Fill in the values. */ newnode->data=data; newnode->filename=filename; if(filename != NULL && gal_fits_name_is_fits(filename)) { /* Set the HDU for this filename. */ if(p->globalhdu) gal_checkset_allocate_copy(p->globalhdu, &newnode->hdu); else newnode->hdu=gal_list_str_pop(&p->hdus); /* Increment the FITS counter. */ ++p->addcounter; } /* Make the link to the previous list. */ newnode->next=p->operands; p->operands=newnode; } } gal_data_t * operands_pop(struct arithmeticparams *p, char *operator) { size_t i; gal_data_t *data; char *filename, *hdu; struct operand *operands=p->operands; /* If the operand linked list has finished, then give an error and exit. */ if(operands==NULL) error(EXIT_FAILURE, 0, "not enough operands for the \"%s\" operator", operator); /* Set the dataset. If filename is present then read the file and fill in the array, if not then just set the array. */ if(operands->filename) { hdu=operands->hdu; filename=operands->filename; /* Read the dataset. */ data=gal_fits_img_read(filename, hdu, p->cp.minmapsize, 0, 0); /* In case this is the first image that is read, then keep the WCS information in the `refdata' structure. Otherwise, the WCS is not necessary and we can safely free it. In any case, `data' must not have a WCS structure. */ if(p->popcounter==0) { p->refdata.wcs=data->wcs; p->refdata.nwcs=data->nwcs; } else wcsfree(data->wcs); data->wcs=NULL; data->nwcs=0; /* When the reference data structure's dimensionality is non-zero, it means that this is not the first image read. So, write its basic information into the reference data structure for future checks. */ if(p->refdata.ndim) { if(gal_data_dsize_is_different(&p->refdata, data)) error(EXIT_FAILURE, 0, "%s (hdu=%s): has a different size " "compared to previous images. All the images must be " "the same size in order for Arithmetic to work", filename, hdu); } else { /* Set the dimensionality. */ p->refdata.ndim=(data)->ndim; /* Allocate the dsize array. */ errno=0; p->refdata.dsize=malloc(p->refdata.ndim * sizeof *p->refdata.dsize); if(p->refdata.dsize==NULL) error(EXIT_FAILURE, errno, "%s: allocating %zu bytes for " "p->refdata.dsize", __func__, p->refdata.ndim * sizeof *p->refdata.dsize); /* Write the values into it. */ for(i=0;i<p->refdata.ndim;++i) p->refdata.dsize[i]=data->dsize[i]; } /* Report the read image if desired: */ if(!p->cp.quiet) printf(" - %s (hdu %s) is read.\n", filename, hdu); /* Free the HDU string: */ free(hdu); /* Add to the number of popped FITS images: */ ++p->popcounter; } else data=operands->data; /* Remove this node from the queue, return the data structure. */ p->operands=operands->next; free(operands); return data; } ������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/arithmetic.c������������������������������������������������������������0000644�0001750�0001750�00000064620�13215601241�015342� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <math.h> #include <stdio.h> #include <errno.h> #include <error.h> #include <string.h> #include <stdlib.h> #include <gnuastro/wcs.h> #include <gnuastro/fits.h> #include <gnuastro/threads.h> #include <gnuastro/dimension.h> #include <gnuastro/statistics.h> #include <gnuastro/arithmetic.h> #include <gnuastro-internal/checkset.h> #include "main.h" #include "operands.h" #include "arithmetic.h" /***************************************************************/ /************* Internal functions *************/ /***************************************************************/ #define SET_NUM_OP(CTYPE) { \ CTYPE a=*(CTYPE *)(data->array); if(a>0) return a; } static size_t pop_number_of_operands(struct arithmeticparams *p, gal_data_t *data, char *token_string) { /* Check if its a number. */ if(data->size>1) error(EXIT_FAILURE, 0, "the first popped operand to the \"%s\" " "operator must be a number, not an array", token_string); /* Check its type and return the value. */ switch(data->type) { /* For the integer types, if they are unsigned, then just pass their value, if they are signed, you have to make sure they are zero or positive. */ case GAL_TYPE_UINT8: SET_NUM_OP(uint8_t); break; case GAL_TYPE_INT8: SET_NUM_OP(int8_t); break; case GAL_TYPE_UINT16: SET_NUM_OP(uint16_t); break; case GAL_TYPE_INT16: SET_NUM_OP(int16_t); break; case GAL_TYPE_UINT32: SET_NUM_OP(uint32_t); break; case GAL_TYPE_INT32: SET_NUM_OP(int32_t); break; case GAL_TYPE_UINT64: SET_NUM_OP(uint64_t); break; case GAL_TYPE_INT64: SET_NUM_OP(int64_t); break; /* Floating point numbers are not acceptable in this context. */ case GAL_TYPE_FLOAT32: case GAL_TYPE_FLOAT64: error(EXIT_FAILURE, 0, "the first popped operand to the \"%s\" " "operator must be an integer type", token_string); default: error(EXIT_FAILURE, 0, "%s: type code %d not recognized", __func__, data->type); } /* If control reaches here, then the number must have been a negative value, so print an error. */ error(EXIT_FAILURE, 0, "the first popped operand to the \"%s\" operator " "cannot be zero or a negative number", token_string); return 0; } /**********************************************************************/ /**************** Filtering operators *****************/ /**********************************************************************/ #define ARITHMETIC_FILTER_DIM 10 struct arithmetic_filter_p { int operator; /* The type of filtering. */ size_t *fsize; /* Filter size. */ size_t *hpfsize; /* Positive Half-filter size. */ size_t *hnfsize; /* Negative Half-filter size. */ gal_data_t *input; /* Input dataset. */ gal_data_t *out; /* Output dataset. */ int hasblank; /* If the dataset has blank values.*/ }; /* Main filtering work function. */ static void * arithmetic_filter(void *in_prm) { struct gal_threads_params *tprm=(struct gal_threads_params *)in_prm; struct arithmetic_filter_p *afp=(struct arithmetic_filter_p *)tprm->params; gal_data_t *input=afp->input; size_t ind,index; int out_type_checked=0; gal_data_t *result=NULL; size_t *hpfsize=afp->hpfsize, *hnfsize=afp->hnfsize; size_t *tsize, *dsize=input->dsize, *fsize=afp->fsize; size_t i, j, coord[ARITHMETIC_FILTER_DIM], ndim=input->ndim; size_t start[ARITHMETIC_FILTER_DIM], end[ARITHMETIC_FILTER_DIM]; gal_data_t *tile=gal_data_alloc(NULL, input->type, ndim, afp->fsize, NULL, 0, -1, NULL, NULL, NULL); /* Prepare the tile. */ free(tile->array); tsize=tile->dsize; tile->block=input; /* Go over all the pixels that were assigned to this thread. */ for(i=0; tprm->indexs[i] != GAL_BLANK_SIZE_T; ++i) { /* Get the coordinate of the pixel. */ ind=tprm->indexs[i]; gal_dimension_index_to_coord(ind, ndim, dsize, coord); /* See which dimensions need trimming. */ tile->size=1; for(j=0;j<ndim;++j) { /* Estimate the coordinate of the filter's starting point. Note that we are dealing with size_t (unsigned int) type here, so there are no negatives. A negative result will produce an extremely large number, so instead of checking for negative, we can just see if the result of a subtraction is less than the width of the input. */ if( (coord[j] - hnfsize[j] > dsize[j]) || (coord[j] + hpfsize[j] >= dsize[j]) ) { start[j] = ( (coord[j] - hnfsize[j] > dsize[j]) ? 0 : coord[j] - hnfsize[j] ); end[j] = ( (coord[j] + hpfsize[j] >= dsize[j]) ? dsize[j] : coord[j] + hpfsize[j] + 1); tsize[j] = end[j] - start[j]; } else /* We are NOT on the edge (given requested filter width). */ { tsize[j] = fsize[j]; start[j] = coord[j] - hnfsize[j]; } tile->size *= tsize[j]; } /* Set the tile's starting pointer. */ index=gal_dimension_coord_to_index(ndim, dsize, start); tile->array=gal_data_ptr_increment(input->array, index, input->type); /* Do the necessary calculation. */ switch(afp->operator) { case ARITHMETIC_OP_FILTER_MEDIAN: result=gal_statistics_median(tile, 0); break; case ARITHMETIC_OP_FILTER_MEAN: result=gal_statistics_mean(tile); break; default: error(EXIT_FAILURE, 0, "%s: a bug! Please contact us at %s to " "fix the problem. `afp->operator' code %d is not " "recognized", PACKAGE_BUGREPORT, __func__, afp->operator); } /* Make sure the output array type and result's type are the same. We only need to do this once, but we'll suffice to once for each thread for simplicify of the code, it is too negligible to have any real affect. */ if( out_type_checked==0) { if(result->type!=afp->out->type ) error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s so " "we can address the problem. The tyes of `result' and " "`out' aren't the same, they are respectively: `%s' and " "`%s'", __func__, PACKAGE_BUGREPORT, gal_type_name(result->type, 1), gal_type_name(afp->out->type, 1)); out_type_checked=1; } /* Copy the result into the output array. */ memcpy(gal_data_ptr_increment(afp->out->array, ind, afp->out->type), result->array, gal_type_sizeof(afp->out->type)); /* Clean up. */ gal_data_free(result); } /* Clean up. */ tile->array=NULL; tile->block=NULL; gal_data_free(tile); /* Wait for all the other threads to finish, then return. */ if(tprm->b) pthread_barrier_wait(tprm->b); return NULL; } static void wrapper_for_filter(struct arithmeticparams *p, char *token, int operator) { size_t i=0, ndim, one=1; int type=GAL_TYPE_INVALID; struct arithmetic_filter_p afp={0}; size_t fsize[ARITHMETIC_FILTER_DIM]; gal_data_t *tmp, *tmp2, *zero, *comp, *fsize_list=NULL; size_t hnfsize[ARITHMETIC_FILTER_DIM], hpfsize[ARITHMETIC_FILTER_DIM]; /* Get the input's number of dimensions. */ afp.input=operands_pop(p, token); afp.operator=operator; ndim=afp.input->ndim; afp.hnfsize=hnfsize; afp.hpfsize=hpfsize; afp.fsize=fsize; /* A small sanity check. */ if(ndim>ARITHMETIC_FILTER_DIM) error(EXIT_FAILURE, 0, "%s: currently only datasets with less than " "%d dimensions are acceptable. The input has %zu dimensions", __func__, ARITHMETIC_FILTER_DIM, ndim); /* A zero value for checking the value of input widths. */ zero=gal_data_alloc(NULL, GAL_TYPE_INT32, 1, &one, NULL, 1, -1, NULL, NULL, NULL); /* Based on the dimensions of the popped operand, pop the necessary number of operands. */ for(i=0;i<ndim;++i) gal_list_data_add(&fsize_list, operands_pop(p, token)); /* Make sure the filter size only has single values. */ i=0; for(tmp=fsize_list; tmp!=NULL; tmp=tmp->next) { ++i; if(tmp->size!=1) error(EXIT_FAILURE, 0, "the filter length values given to the " "filter operators can only be numbers. Value number %zu has " "%zu elements, so its an array", ndim-i-1, tmp->size); } /* If the input only has one element, filtering makes no sense, so don't waste time, just add the input onto the stack. */ if(afp.input->size==1) afp.out=afp.input; else { /* Allocate an array for the size of the filter and fill it in. The values must be written in the inverse order since the user gives dimensions with the FITS standard. */ i=ndim-1; for(tmp=fsize_list; tmp!=NULL; tmp=tmp->next) { /* Make sure the user has given an integer type. */ if(tmp->type==GAL_TYPE_FLOAT32 || tmp->type==GAL_TYPE_FLOAT64) error(EXIT_FAILURE, 0, "lengths of filter along dimensions " "must be integer values, not floats. The given length " "along dimension %zu is a float", ndim-i); /* Make sure it isn't negative. */ comp=gal_arithmetic(GAL_ARITHMETIC_OP_GT, 0, tmp, zero); if( *(uint8_t *)(comp->array) == 0 ) error(EXIT_FAILURE, 0, "lengths of filter along dimensions " "must be positive. The given length in dimension %zu" "is either zero or negative", ndim-i); /* Convert the input into size_t and put it into the array that keeps the filter size. */ tmp2=gal_data_copy_to_new_type(tmp, GAL_TYPE_SIZE_T); fsize[ i ] = *(size_t *)(tmp2->array); gal_data_free(tmp2); /* If the width is larger than the input's size, change the width to the input's size. */ if( fsize[i] > afp.input->dsize[i] ) error(EXIT_FAILURE, 0, "%s: the filter size along dimension %zu " "(%zu) is greater than the input's length in that " "dimension (%zu)", __func__, i, fsize[i], afp.input->dsize[i]); /* Go onto the previous dimension. */ --i; } /* Set the half filter sizes. Note that when the size is an odd number, the number of pixels before and after the actual pixel are equal, but for an even number, we will look into one element more when looking before than the ones after. */ for(i=0;i<ndim;++i) { if( fsize[i]%2 ) hnfsize[i]=hpfsize[i]=fsize[i]/2; else { hnfsize[i]=fsize[i]/2; hpfsize[i]=fsize[i]/2-1; } } /* See if the input has blank pixels. */ afp.hasblank=gal_blank_present(afp.input, 1); /* Set the type of the output dataset. */ switch(operator) { case ARITHMETIC_OP_FILTER_MEDIAN: type=afp.input->type; break; case ARITHMETIC_OP_FILTER_MEAN: type=GAL_TYPE_FLOAT64; break; default: error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to fix " "the problem. The `operator' code %d is not recognized", PACKAGE_BUGREPORT, __func__, operator); } /* Allocate the output dataset. Note that filtering doesn't change the units of the dataset. */ afp.out=gal_data_alloc(NULL, type, ndim, afp.input->dsize, afp.input->wcs, 0, afp.input->minmapsize, NULL, afp.input->unit, NULL); /* Spin off threads for each pixel. */ gal_threads_spin_off(arithmetic_filter, &afp, afp.input->size, p->cp.numthreads); } /* Add the output to the top of the stack. */ operands_add(p, NULL, afp.out); /* Clean up and add the output on top of the stack */ gal_data_free(afp.input); gal_list_data_free(fsize_list); } /***************************************************************/ /************* Reverse Polish algorithm *************/ /***************************************************************/ /* This function implements the reverse polish algorithm as explained in the Wikipedia page. NOTE that in ui.c, the input linked list of tokens was ordered to have the same order as what the user provided. */ void reversepolish(struct arithmeticparams *p) { int op=0, nop=0; char *filename, *hdu; unsigned int numop, i; gal_list_str_t *token; gal_data_t *d1=NULL, *d2=NULL, *d3=NULL; int flags = ( GAL_ARITHMETIC_INPLACE | GAL_ARITHMETIC_FREE | GAL_ARITHMETIC_NUMOK ); /* Prepare the processing: */ p->operands=NULL; p->addcounter=p->popcounter=0; /* Go over each input token and do the work. */ for(token=p->tokens;token!=NULL;token=token->next) { /* If we have a name or number, then add it to the operands linked list. Otherwise, pull out two members and do the specified operation on them. */ if(gal_fits_name_is_fits(token->v)) operands_add(p, token->v, NULL); else if( (d1=gal_data_copy_string_to_number(token->v)) ) operands_add(p, NULL, d1); else { /* Order is the same as in the manual. */ /* Simple arithmetic operators. */ if (!strcmp(token->v, "+" )) { op=GAL_ARITHMETIC_OP_PLUS; nop=2; } else if (!strcmp(token->v, "-" )) { op=GAL_ARITHMETIC_OP_MINUS; nop=2; } else if (!strcmp(token->v, "x" )) { op=GAL_ARITHMETIC_OP_MULTIPLY; nop=2; } else if (!strcmp(token->v, "/" )) { op=GAL_ARITHMETIC_OP_DIVIDE; nop=2; } else if (!strcmp(token->v, "%" )) { op=GAL_ARITHMETIC_OP_MODULO; nop=2; } /* Mathematical Operators. */ else if (!strcmp(token->v, "abs")) { op=GAL_ARITHMETIC_OP_ABS; nop=1; } else if (!strcmp(token->v, "pow")) { op=GAL_ARITHMETIC_OP_POW; nop=2; } else if (!strcmp(token->v, "sqrt")) { op=GAL_ARITHMETIC_OP_SQRT; nop=1; } else if (!strcmp(token->v, "log")) { op=GAL_ARITHMETIC_OP_LOG; nop=1; } else if (!strcmp(token->v, "log10")) { op=GAL_ARITHMETIC_OP_LOG10; nop=1; } /* Statistical/higher-level operators. */ else if (!strcmp(token->v, "minvalue")) { op=GAL_ARITHMETIC_OP_MINVAL; nop=1; } else if (!strcmp(token->v, "maxvalue")) { op=GAL_ARITHMETIC_OP_MAXVAL; nop=1; } else if (!strcmp(token->v, "numvalue")) { op=GAL_ARITHMETIC_OP_NUMVAL; nop=1; } else if (!strcmp(token->v, "sumvalue")) { op=GAL_ARITHMETIC_OP_SUMVAL; nop=1; } else if (!strcmp(token->v, "meanvalue")) { op=GAL_ARITHMETIC_OP_MEANVAL; nop=1; } else if (!strcmp(token->v, "stdvalue")) { op=GAL_ARITHMETIC_OP_STDVAL; nop=1; } else if (!strcmp(token->v, "medianvalue")) { op=GAL_ARITHMETIC_OP_MEDIANVAL; nop=1; } else if (!strcmp(token->v, "min")) { op=GAL_ARITHMETIC_OP_MIN; nop=-1; } else if (!strcmp(token->v, "max")) { op=GAL_ARITHMETIC_OP_MAX; nop=-1; } else if (!strcmp(token->v, "num")) { op=GAL_ARITHMETIC_OP_NUM; nop=-1; } else if (!strcmp(token->v, "sum")) { op=GAL_ARITHMETIC_OP_SUM; nop=-1; } else if (!strcmp(token->v, "mean")) { op=GAL_ARITHMETIC_OP_MEAN; nop=-1; } else if (!strcmp(token->v, "std")) { op=GAL_ARITHMETIC_OP_STD; nop=-1; } else if (!strcmp(token->v, "median")) { op=GAL_ARITHMETIC_OP_MEDIAN; nop=-1; } /* Conditional operators. */ else if (!strcmp(token->v, "lt" )) { op=GAL_ARITHMETIC_OP_LT; nop=2; } else if (!strcmp(token->v, "le")) { op=GAL_ARITHMETIC_OP_LE; nop=2; } else if (!strcmp(token->v, "gt" )) { op=GAL_ARITHMETIC_OP_GT; nop=2; } else if (!strcmp(token->v, "ge")) { op=GAL_ARITHMETIC_OP_GE; nop=2; } else if (!strcmp(token->v, "eq")) { op=GAL_ARITHMETIC_OP_EQ; nop=2; } else if (!strcmp(token->v, "ne")) { op=GAL_ARITHMETIC_OP_NE; nop=2; } else if (!strcmp(token->v, "and")) { op=GAL_ARITHMETIC_OP_AND; nop=2; } else if (!strcmp(token->v, "or")) { op=GAL_ARITHMETIC_OP_OR; nop=2; } else if (!strcmp(token->v, "not")) { op=GAL_ARITHMETIC_OP_NOT; nop=1; } else if (!strcmp(token->v, "isblank")) { op=GAL_ARITHMETIC_OP_ISBLANK; nop=1; } else if (!strcmp(token->v, "where")) { op=GAL_ARITHMETIC_OP_WHERE; nop=3; } /* Bitwise operators. */ else if (!strcmp(token->v, "bitand")) { op=GAL_ARITHMETIC_OP_BITAND; nop=2; } else if (!strcmp(token->v, "bitor")) { op=GAL_ARITHMETIC_OP_BITOR; nop=2; } else if (!strcmp(token->v, "bitxor")) { op=GAL_ARITHMETIC_OP_BITXOR; nop=2; } else if (!strcmp(token->v, "lshift")) { op=GAL_ARITHMETIC_OP_BITLSH; nop=2; } else if (!strcmp(token->v, "rshift")) { op=GAL_ARITHMETIC_OP_BITRSH; nop=2; } else if (!strcmp(token->v, "bitnot")) { op=GAL_ARITHMETIC_OP_BITNOT; nop=1; } /* Type conversion. */ else if (!strcmp(token->v, "uint8")) { op=GAL_ARITHMETIC_OP_TO_UINT8; nop=1; } else if (!strcmp(token->v, "int8")) { op=GAL_ARITHMETIC_OP_TO_INT8; nop=1; } else if (!strcmp(token->v, "uint16")) { op=GAL_ARITHMETIC_OP_TO_UINT16; nop=1; } else if (!strcmp(token->v, "int16")) { op=GAL_ARITHMETIC_OP_TO_INT16; nop=1; } else if (!strcmp(token->v, "uint32")) { op=GAL_ARITHMETIC_OP_TO_UINT32; nop=1; } else if (!strcmp(token->v, "int32")) { op=GAL_ARITHMETIC_OP_TO_INT32; nop=1; } else if (!strcmp(token->v, "uint64")) { op=GAL_ARITHMETIC_OP_TO_UINT64; nop=1; } else if (!strcmp(token->v, "int64")) { op=GAL_ARITHMETIC_OP_TO_INT64; nop=1; } else if (!strcmp(token->v, "float32")) { op=GAL_ARITHMETIC_OP_TO_FLOAT32; nop=1; } else if (!strcmp(token->v, "float64")) { op=GAL_ARITHMETIC_OP_TO_FLOAT64; nop=1; } /* Filters. */ else if (!strcmp(token->v, "filter-median")) { op=ARITHMETIC_OP_FILTER_MEDIAN; nop=0; } else if (!strcmp(token->v, "filter-mean")) { op=ARITHMETIC_OP_FILTER_MEAN; nop=0; } /* Finished checks with known operators */ else error(EXIT_FAILURE, 0, "the argument \"%s\" could not be " "interpretted as a FITS file, number, or operator", token->v); /* See if the arithmetic library must be called or not. */ if(nop) { /* Pop the necessary number of operators. Note that the operators are poped from a linked list (which is last-in-first-out). So for the operators which need a specific order, the first poped operand is actally the last (right most, in in-fix notation) input operand.*/ switch(nop) { case 1: d1=operands_pop(p, token->v); break; case 2: d2=operands_pop(p, token->v); d1=operands_pop(p, token->v); break; case 3: d3=operands_pop(p, token->v); d2=operands_pop(p, token->v); d1=operands_pop(p, token->v); break; case -1: /* This case is when the number of operands is itself an operand. So the first popped operand must be an integer number, we will use that to construct a linked list of any number of operands within the single `d1' pointer. */ d1=NULL; numop=pop_number_of_operands(p, operands_pop(p, token->v), token->v); for(i=0;i<numop;++i) gal_list_data_add(&d1, operands_pop(p, token->v)); break; default: error(EXIT_FAILURE, 0, "no operators, `%s' needs %d " "operand(s)", token->v, nop); } /* Run the arithmetic operation. Note that `gal_arithmetic' is a variable argument function (like printf). So the number of arguments it uses depend on the operator. So when the operator doesn't need three operands, the extra arguments will be ignored. */ operands_add(p, NULL, gal_arithmetic(op, flags, d1, d2, d3)); } /* No need to call the arithmetic library, call the proper wrappers directly. */ else { switch(op) { case ARITHMETIC_OP_FILTER_MEAN: case ARITHMETIC_OP_FILTER_MEDIAN: wrapper_for_filter(p, token->v, op); break; default: error(EXIT_FAILURE, 0, "%s: a bug! please contact us at " "%s to fix the problem. The code %d is not " "recognized for `op'", __func__, PACKAGE_BUGREPORT, op); } } } } /* If there is more than one node in the operands stack then the user has given too many operands which is an error. */ if(p->operands->next!=NULL) error(EXIT_FAILURE, 0, "too many operands"); /* If the final operand has a filename, but its `data' element is NULL, then the file hasn't actually be read yet. In this case, we need to read the contents of the file and put the resulting dataset into the operands `data' element. This can happen for example if no operators are called and there is only one filename as an argument (which can happen in scripts). */ if(p->operands->data==NULL && p->operands->filename) { /* Read the desired image and report it if necessary. */ hdu=p->operands->hdu; filename=p->operands->filename; if( gal_fits_name_is_fits(filename) ) { p->operands->data=gal_fits_img_read(filename,hdu,p->cp.minmapsize, 0, 0); p->refdata.wcs=p->operands->data->wcs; p->refdata.nwcs=p->operands->data->nwcs; p->operands->data->wcs=NULL; if(!p->cp.quiet) printf(" - %s (hdu %s) is read.\n", filename, hdu); } else error(EXIT_FAILURE, 0, "%s: a bug! please contact us at %s to fix " "the problem. While `operands->data' is NULL, the filename " "(`%s') is not recognized as a FITS file", __func__, PACKAGE_BUGREPORT, filename); } /* If the final data structure has more than one element, write it as a FITS file. Otherwise, print it in the standard output. */ d1=p->operands->data; if(d1->size==1) { /* To simplify the printing process, we will first change it to double, then use printf's `%g' to print it, so integers will be printed as an integer. */ d2=gal_data_copy_to_new_type(d1, GAL_TYPE_FLOAT64); printf("%g\n", *(double *)d2->array); if(d2!=d1) gal_data_free(d2); } else { /* Put a copy of the WCS structure from the reference image, it will be freed while freeing d1. */ d1->wcs=p->refdata.wcs; gal_fits_img_write(d1, p->cp.output, NULL, PROGRAM_NAME); if(!p->cp.quiet) printf(" - Output written to %s\n", p->cp.output); } /* Clean up, note that above, we copied the pointer to `refdata->wcs' into `d1', so it is freed when freeing d1. */ gal_data_free(d1); free(p->refdata.dsize); /* Clean up. Note that the tokens were taken from the command-line arguments, so the string within each token linked list must not be freed. */ gal_list_str_free(p->tokens, 0); free(p->operands); } /***************************************************************/ /************* Top function *************/ /***************************************************************/ void imgarith(struct arithmeticparams *p) { /* Parse the arguments */ reversepolish(p); } ����������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/ui.c��������������������������������������������������������������������0000644�0001750�0001750�00000030502�13211076737�013632� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <argp.h> #include <errno.h> #include <error.h> #include <stdio.h> #include <gnuastro/list.h> #include <gnuastro/fits.h> #include <gnuastro/table.h> #include <gnuastro-internal/timing.h> #include <gnuastro-internal/options.h> #include <gnuastro-internal/checkset.h> #include <gnuastro-internal/fixedstringmacros.h> #include "main.h" #include "ui.h" #include "authors-cite.h" /**************************************************************/ /********* Argp necessary global entities ************/ /**************************************************************/ /* Definition parameters for the argp: */ const char * argp_program_version = PROGRAM_STRING "\n" GAL_STRINGS_COPYRIGHT "\n\nWritten/developed by "PROGRAM_AUTHORS; const char * argp_program_bug_address = PACKAGE_BUGREPORT; static char args_doc[] = "ASTRdata or number [ASTRdata] OPERATOR ..."; const char doc[] = GAL_STRINGS_TOP_HELP_INFO PROGRAM_NAME" will do arithmetic " "operations on one or multiple images and numbers. Simply put, the name " "of the image along with the arithmetic operators and possible numbers " "are given as arguments. The extensions of each input are specified with " "(possibly multiple) calls to the `--hdu' option." "\n\nCurrently "PROGRAM_NAME" only supports postfix or reverse polish " "notation. For example to get the result of `5+6', you should write " "`5 6 +', or to get the average of two images, you should write `a.fits " "b.fits + 2 /' (or more simply use the `average' operator with " "`a.fits b.fits average'). Please see the manual for more information. " "\n\n"PROGRAM_NAME" recognizes a large collection of standard operators, " "including basic arithmetic (e.g., +, -, x, /), mathematical (e.g., abs, " "pow, sqrt, log), statistical (minvalue, min, max, average), comparison " "(e.g., lt, le, gt), logical (e.g., and, or, not), the full set of bitwise " "operators, and numeric type conversion operators to all known types. " "Please run the command below for a complete list describing all " "operators (press the `SPACE' keyboard key, or arrow keys, to go down " "and `q' to return to the command-line):\n\n" " $ info gnuastro \"Arithmetic operators\"\n" GAL_STRINGS_MORE_HELP_INFO /* After the list of options: */ "\v" PACKAGE_NAME" home page: "PACKAGE_URL; /**************************************************************/ /********* Initialize & Parse command-line **************/ /**************************************************************/ static void ui_initialize_options(struct arithmeticparams *p, struct argp_option *program_options, struct argp_option *gal_commonopts_options) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Set the necessary common parameters structure. */ cp->poptions = program_options; cp->program_name = PROGRAM_NAME; cp->program_exec = PROGRAM_EXEC; cp->program_bibtex = PROGRAM_BIBTEX; cp->program_authors = PROGRAM_AUTHORS; cp->coptions = gal_commonopts_options; /* Modify the common options. */ for(i=0; !gal_options_is_last(&cp->coptions[i]); ++i) { /* Select individually. */ switch(cp->coptions[i].key) { case GAL_OPTIONS_KEY_HDU: cp->coptions[i].value=&p->hdus; cp->coptions[i].type=GAL_TYPE_STRLL; cp->coptions[i].doc="Nth call, used for HDU of Nth input FITS."; break; case GAL_OPTIONS_KEY_TYPE: case GAL_OPTIONS_KEY_SEARCHIN: case GAL_OPTIONS_KEY_IGNORECASE: case GAL_OPTIONS_KEY_TABLEFORMAT: cp->coptions[i].flags=OPTION_HIDDEN; break; case GAL_OPTIONS_KEY_MINMAPSIZE: cp->coptions[i].mandatory=GAL_OPTIONS_MANDATORY; break; } /* Select by group. */ switch(cp->coptions[i].group) { case GAL_OPTIONS_GROUP_TESSELLATION: cp->coptions[i].doc=NULL; /* Necessary to remove title. */ cp->coptions[i].flags=OPTION_HIDDEN; break; } } } /* Parse a single option: */ error_t parse_opt(int key, char *arg, struct argp_state *state) { struct arithmeticparams *p = state->input; /* Pass `gal_options_common_params' into the child parser. */ state->child_inputs[0] = &p->cp; /* In case the user incorrectly uses the equal sign (for example with a short format or with space in the long format, then `arg` start with (if the short version was called) or be (if the long version was called with a space) the equal sign. So, here we check if the first character of arg is the equal sign, then the user is warned and the program is stopped: */ if(arg && arg[0]=='=') argp_error(state, "incorrect use of the equal sign (`=`). For short " "options, `=` should not be used and for long options, " "there should be no space between the option, equal sign " "and value"); /* Set the key to this option. */ switch(key) { /* Read the non-option tokens (arguments): */ case ARGP_KEY_ARG: gal_list_str_add(&p->tokens, arg, 0); break; /* This is an option, set its value. */ default: return gal_options_set_from_key(key, arg, p->cp.poptions, &p->cp); } return 0; } /**************************************************************/ /*************** Sanity Check *******************/ /**************************************************************/ /* Sanity check on options AND arguments. If only option values are to be checked, use `ui_read_check_only_options'. */ static void ui_check_options_and_arguments(struct arithmeticparams *p) { int output_checked=0; size_t numfits=0, numhdus=0; gal_list_str_t *token, *hdu; /* First, make sure that any tokens are actually given. */ if(p->tokens==NULL) error(EXIT_FAILURE, 0, "no input tokens. Please specify a filename or " "number (as operands) along with operator(s) as input. Please run " "any of the following commands for more information.\n\n" " $ astarithmetic --help # Short info.\n" " $ info astarithmetic # Full invocation " "documentation.\n"); /* The input tokens are put in a lastin-firstout (simple) linked list, so change them to the correct order so the order we pop a token is the same order that the user input a value. Note that for the options this was done in `gal_options_read_config_set'. */ gal_list_str_reverse(&p->tokens); /* Set the output file name (if any is needed). Note that since the lists are already reversed, the first FITS file encountered, is the first FITS file given by teh user. Also, notet that these file name operations are only necessary for the first FITS file in the token list. */ for(token=p->tokens; token!=NULL; token=token->next) { /* This token is a FITS file, count them and use it to set the output filename if it has not been set. */ if(gal_fits_name_is_fits(token->v)) { /* Increment the counter for FITS files. */ ++numfits; /* If the output filename isn't set yet, then set it. */ if(output_checked==0) { if(p->cp.output) gal_checkset_writable_remove(p->cp.output, 0, p->cp.dontdelete); else p->cp.output=gal_checkset_automatic_output(&p->cp, token->v, "_arith.fits"); output_checked=1; } } /* This token is a number. Check if a negative dash was present that has been temporarily replaced with `NEG_DASH_REPLACE' before option parsing. */ else if(token->v[0]==NEG_DASH_REPLACE && isdigit(token->v[1]) ) token->v[0]='-'; } /* Count the number of HDU values (if globalhdu isn't given) and check if its not less than the number of input FITS images. */ if(p->globalhdu) { if(p->hdus) { gal_list_str_free(p->hdus, 1); p->hdus=NULL; }; } else { for(hdu=p->hdus; hdu!=NULL; hdu=hdu->next) ++numhdus; if(numhdus<numfits) error(EXIT_FAILURE, 0, "not enough HDUs. There are %zu input FITS " "files, so the `--hdu' (`-h') option must be called %zu " "times (once for each FITS file). If the HDU value is the " "same for all the files, you may use `--globalhdu' (`-g') to " "specify a single HDU to be used for any number of input " "files", numfits, numfits); } } /**************************************************************/ /************ Set the parameters *************/ /**************************************************************/ void ui_read_check_inputs_setup(int argc, char *argv[], struct arithmeticparams *p) { size_t i; struct gal_options_common_params *cp=&p->cp; /* Include the parameters necessary for argp from this program (`args.h') and for the common options to all Gnuastro (`commonopts.h'). We want to directly put the pointers to the fields in `p' and `cp', so we are simply including the header here to not have to use long macros in those headers which make them hard to read and modify. This also helps in having a clean environment: everything in those headers is only available within the scope of this function. */ #include <gnuastro-internal/commonopts.h> #include "args.h" /* Initialize the options and necessary information. */ ui_initialize_options(p, program_options, gal_commonopts_options); /* The dash of a negative number will cause problems with the option readin. To work properly we will go over all the options/arguments and if any one starts with a dash and is followed by a number, then the dash is replaced by NEG_DASH_REPLACE. */ for(i=0;i<argc;++i) if(argv[i][0]=='-' && isdigit(argv[i][1])) argv[i][0]=NEG_DASH_REPLACE; /* Read the command-line options and arguments. */ errno=0; if(argp_parse(&thisargp, argc, argv, 0, 0, p)) error(EXIT_FAILURE, errno, "parsing arguments"); /* Read the configuration files. */ gal_options_read_config_set(cp); /* Print the option values if asked. Note that this needs to be done after the sanity check so un-sane values are not printed in the output state. */ gal_options_print_state(cp); /* Check that the options and arguments fit well with each other. Note that arguments don't go in a configuration file. So this test should be done after (possibly) printing the option values. */ ui_check_options_and_arguments(p); } /**************************************************************/ /************ Free allocated, report *************/ /**************************************************************/ void freeandreport(struct arithmeticparams *p, struct timeval *t1) { /* Free the simple strings. */ free(p->cp.output); if(p->globalhdu) free(p->globalhdu); /* If there are any remaining HDUs in the hdus linked list, then free them. */ if(p->hdus) gal_list_str_free(p->hdus, 1); /* Report the duration of the job */ if(!p->cp.quiet) gal_timing_report(t1, PROGRAM_NAME" finished in", 0); } ����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/main.c������������������������������������������������������������������0000644�0001750�0001750�00000003167�13121462410�014133� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������/********************************************************************* Arithmetic - Do arithmetic operations on images. Arithmetic is part of GNU Astronomy Utilities (Gnuastro) package. Original author: Mohammad Akhlaghi <akhlaghi@gnu.org> Contributing author(s): Copyright (C) 2015, Free Software Foundation, Inc. Gnuastro is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. Gnuastro is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. **********************************************************************/ #include <config.h> #include <stdio.h> #include <stdlib.h> #include <gnuastro-internal/timing.h> #include "main.h" #include "ui.h" /* needs main.h. */ #include "arithmetic.h" /* needs main.h. */ int main (int argc, char *argv[]) { struct timeval t1; struct arithmeticparams p={{{0},0},0}; /* Set the starting time. */ time(&p.rawtime); gettimeofday(&t1, NULL); /* Read the input parameters. */ ui_read_check_inputs_setup(argc, argv, &p); /* Run MakeProfiles */ imgarith(&p); /* Free any allocated space */ freeandreport(&p, &t1); /* Return successfully.*/ return 0; } ���������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/Makefile.in�������������������������������������������������������������0000644�0001750�0001750�00000211625�13217217705�015123� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Makefile.in generated by automake 1.15.1 from Makefile.am. # @configure_input@ # Copyright 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GNULIB_LOGB = @GNULIB_LOGB@ GNULIB_LOGBF = @GNULIB_LOGBF@ GNULIB_LOGBL = @GNULIB_LOGBL@ GNULIB_LOGF = @GNULIB_LOGF@ GNULIB_LOGL = @GNULIB_LOGL@ GNULIB_LSEEK = @GNULIB_LSEEK@ GNULIB_LSTAT = @GNULIB_LSTAT@ GNULIB_MALLOC_POSIX = @GNULIB_MALLOC_POSIX@ GNULIB_MBRLEN = @GNULIB_MBRLEN@ GNULIB_MBRTOWC = @GNULIB_MBRTOWC@ GNULIB_MBSCASECMP = @GNULIB_MBSCASECMP@ GNULIB_MBSCASESTR = @GNULIB_MBSCASESTR@ GNULIB_MBSCHR = @GNULIB_MBSCHR@ GNULIB_MBSCSPN = @GNULIB_MBSCSPN@ GNULIB_MBSINIT = @GNULIB_MBSINIT@ GNULIB_MBSLEN = @GNULIB_MBSLEN@ GNULIB_MBSNCASECMP = @GNULIB_MBSNCASECMP@ GNULIB_MBSNLEN = @GNULIB_MBSNLEN@ GNULIB_MBSNRTOWCS = @GNULIB_MBSNRTOWCS@ GNULIB_MBSPBRK = @GNULIB_MBSPBRK@ GNULIB_MBSPCASECMP = @GNULIB_MBSPCASECMP@ GNULIB_MBSRCHR = @GNULIB_MBSRCHR@ GNULIB_MBSRTOWCS = @GNULIB_MBSRTOWCS@ GNULIB_MBSSEP = @GNULIB_MBSSEP@ GNULIB_MBSSPN = @GNULIB_MBSSPN@ GNULIB_MBSSTR = @GNULIB_MBSSTR@ GNULIB_MBSTOK_R = @GNULIB_MBSTOK_R@ GNULIB_MBTOWC = @GNULIB_MBTOWC@ GNULIB_MEMCHR = @GNULIB_MEMCHR@ GNULIB_MEMMEM = @GNULIB_MEMMEM@ GNULIB_MEMPCPY = @GNULIB_MEMPCPY@ GNULIB_MEMRCHR = @GNULIB_MEMRCHR@ GNULIB_MKDIRAT = @GNULIB_MKDIRAT@ GNULIB_MKDTEMP = @GNULIB_MKDTEMP@ GNULIB_MKFIFO = @GNULIB_MKFIFO@ GNULIB_MKFIFOAT = @GNULIB_MKFIFOAT@ GNULIB_MKNOD = @GNULIB_MKNOD@ GNULIB_MKNODAT = @GNULIB_MKNODAT@ GNULIB_MKOSTEMP = @GNULIB_MKOSTEMP@ GNULIB_MKOSTEMPS = @GNULIB_MKOSTEMPS@ GNULIB_MKSTEMP = @GNULIB_MKSTEMP@ GNULIB_MKSTEMPS = @GNULIB_MKSTEMPS@ GNULIB_MKTIME = @GNULIB_MKTIME@ GNULIB_MODF = @GNULIB_MODF@ GNULIB_MODFF = @GNULIB_MODFF@ GNULIB_MODFL = @GNULIB_MODFL@ GNULIB_NANOSLEEP = @GNULIB_NANOSLEEP@ GNULIB_NL_LANGINFO = @GNULIB_NL_LANGINFO@ GNULIB_NONBLOCKING = @GNULIB_NONBLOCKING@ GNULIB_OBSTACK_PRINTF = @GNULIB_OBSTACK_PRINTF@ GNULIB_OBSTACK_PRINTF_POSIX = @GNULIB_OBSTACK_PRINTF_POSIX@ GNULIB_OPEN = @GNULIB_OPEN@ GNULIB_OPENAT = @GNULIB_OPENAT@ GNULIB_OVERRIDES_STRUCT_STAT = @GNULIB_OVERRIDES_STRUCT_STAT@ GNULIB_OVERRIDES_WINT_T = @GNULIB_OVERRIDES_WINT_T@ GNULIB_PCLOSE = @GNULIB_PCLOSE@ GNULIB_PERROR = @GNULIB_PERROR@ GNULIB_PIPE = @GNULIB_PIPE@ GNULIB_PIPE2 = @GNULIB_PIPE2@ GNULIB_POPEN = @GNULIB_POPEN@ GNULIB_POSIX_OPENPT = @GNULIB_POSIX_OPENPT@ GNULIB_POWF = @GNULIB_POWF@ GNULIB_PREAD = @GNULIB_PREAD@ GNULIB_PRINTF = @GNULIB_PRINTF@ GNULIB_PRINTF_POSIX = @GNULIB_PRINTF_POSIX@ GNULIB_PSELECT = @GNULIB_PSELECT@ GNULIB_PTHREAD_SIGMASK = @GNULIB_PTHREAD_SIGMASK@ GNULIB_PTSNAME = @GNULIB_PTSNAME@ GNULIB_PTSNAME_R = @GNULIB_PTSNAME_R@ GNULIB_PUTC = @GNULIB_PUTC@ GNULIB_PUTCHAR = @GNULIB_PUTCHAR@ GNULIB_PUTENV = @GNULIB_PUTENV@ GNULIB_PUTS = @GNULIB_PUTS@ GNULIB_PWRITE = @GNULIB_PWRITE@ GNULIB_QSORT_R = @GNULIB_QSORT_R@ GNULIB_RAISE = @GNULIB_RAISE@ GNULIB_RANDOM = @GNULIB_RANDOM@ GNULIB_RANDOM_R = @GNULIB_RANDOM_R@ GNULIB_RAWMEMCHR = @GNULIB_RAWMEMCHR@ GNULIB_READ = @GNULIB_READ@ GNULIB_READLINK = @GNULIB_READLINK@ GNULIB_READLINKAT = @GNULIB_READLINKAT@ GNULIB_REALLOCARRAY = @GNULIB_REALLOCARRAY@ GNULIB_REALLOC_POSIX = @GNULIB_REALLOC_POSIX@ GNULIB_REALPATH = @GNULIB_REALPATH@ GNULIB_RECV = @GNULIB_RECV@ GNULIB_RECVFROM = @GNULIB_RECVFROM@ GNULIB_REMAINDER = @GNULIB_REMAINDER@ GNULIB_REMAINDERF = @GNULIB_REMAINDERF@ GNULIB_REMAINDERL = @GNULIB_REMAINDERL@ GNULIB_REMOVE = @GNULIB_REMOVE@ GNULIB_RENAME = @GNULIB_RENAME@ GNULIB_RENAMEAT = @GNULIB_RENAMEAT@ GNULIB_RINT = @GNULIB_RINT@ GNULIB_RINTF = @GNULIB_RINTF@ GNULIB_RINTL = @GNULIB_RINTL@ GNULIB_RMDIR = @GNULIB_RMDIR@ GNULIB_ROUND = @GNULIB_ROUND@ GNULIB_ROUNDF = @GNULIB_ROUNDF@ GNULIB_ROUNDL = @GNULIB_ROUNDL@ GNULIB_RPMATCH = @GNULIB_RPMATCH@ GNULIB_SCANF = @GNULIB_SCANF@ GNULIB_SECURE_GETENV = @GNULIB_SECURE_GETENV@ GNULIB_SELECT = @GNULIB_SELECT@ GNULIB_SEND = @GNULIB_SEND@ GNULIB_SENDTO = @GNULIB_SENDTO@ GNULIB_SETENV = @GNULIB_SETENV@ GNULIB_SETHOSTNAME = @GNULIB_SETHOSTNAME@ GNULIB_SETLOCALE = @GNULIB_SETLOCALE@ GNULIB_SETSOCKOPT = @GNULIB_SETSOCKOPT@ GNULIB_SHUTDOWN = @GNULIB_SHUTDOWN@ GNULIB_SIGACTION = @GNULIB_SIGACTION@ GNULIB_SIGNAL_H_SIGPIPE = @GNULIB_SIGNAL_H_SIGPIPE@ GNULIB_SIGNBIT = @GNULIB_SIGNBIT@ GNULIB_SIGPROCMASK = @GNULIB_SIGPROCMASK@ GNULIB_SINF = @GNULIB_SINF@ GNULIB_SINHF = @GNULIB_SINHF@ GNULIB_SINL = @GNULIB_SINL@ GNULIB_SLEEP = @GNULIB_SLEEP@ GNULIB_SNPRINTF = @GNULIB_SNPRINTF@ GNULIB_SOCKET = @GNULIB_SOCKET@ GNULIB_SPRINTF_POSIX = @GNULIB_SPRINTF_POSIX@ GNULIB_SQRTF = @GNULIB_SQRTF@ GNULIB_SQRTL = @GNULIB_SQRTL@ GNULIB_STAT = @GNULIB_STAT@ GNULIB_STDIO_H_NONBLOCKING = @GNULIB_STDIO_H_NONBLOCKING@ GNULIB_STDIO_H_SIGPIPE = @GNULIB_STDIO_H_SIGPIPE@ GNULIB_STPCPY = @GNULIB_STPCPY@ GNULIB_STPNCPY = @GNULIB_STPNCPY@ GNULIB_STRCASESTR = @GNULIB_STRCASESTR@ GNULIB_STRCHRNUL = @GNULIB_STRCHRNUL@ GNULIB_STRDUP = @GNULIB_STRDUP@ GNULIB_STRERROR = @GNULIB_STRERROR@ GNULIB_STRERROR_R = @GNULIB_STRERROR_R@ GNULIB_STRFTIME = @GNULIB_STRFTIME@ GNULIB_STRNCAT = @GNULIB_STRNCAT@ GNULIB_STRNDUP = @GNULIB_STRNDUP@ GNULIB_STRNLEN = @GNULIB_STRNLEN@ GNULIB_STRPBRK = @GNULIB_STRPBRK@ GNULIB_STRPTIME = @GNULIB_STRPTIME@ GNULIB_STRSEP = @GNULIB_STRSEP@ GNULIB_STRSIGNAL = @GNULIB_STRSIGNAL@ GNULIB_STRSTR = @GNULIB_STRSTR@ GNULIB_STRTOD = @GNULIB_STRTOD@ GNULIB_STRTOIMAX = @GNULIB_STRTOIMAX@ GNULIB_STRTOK_R = @GNULIB_STRTOK_R@ GNULIB_STRTOLL = @GNULIB_STRTOLL@ GNULIB_STRTOULL = @GNULIB_STRTOULL@ GNULIB_STRTOUMAX = @GNULIB_STRTOUMAX@ GNULIB_STRVERSCMP = @GNULIB_STRVERSCMP@ GNULIB_SYMLINK = @GNULIB_SYMLINK@ GNULIB_SYMLINKAT = @GNULIB_SYMLINKAT@ GNULIB_SYSTEM_POSIX = @GNULIB_SYSTEM_POSIX@ GNULIB_TANF = @GNULIB_TANF@ GNULIB_TANHF = @GNULIB_TANHF@ GNULIB_TANL = @GNULIB_TANL@ GNULIB_TIMEGM = @GNULIB_TIMEGM@ GNULIB_TIME_R = @GNULIB_TIME_R@ GNULIB_TIME_RZ = @GNULIB_TIME_RZ@ GNULIB_TMPFILE = @GNULIB_TMPFILE@ GNULIB_TOWCTRANS = @GNULIB_TOWCTRANS@ GNULIB_TRUNC = @GNULIB_TRUNC@ GNULIB_TRUNCATE = @GNULIB_TRUNCATE@ GNULIB_TRUNCF = @GNULIB_TRUNCF@ GNULIB_TRUNCL = @GNULIB_TRUNCL@ GNULIB_TTYNAME_R = @GNULIB_TTYNAME_R@ GNULIB_TZSET = @GNULIB_TZSET@ GNULIB_UNISTD_H_NONBLOCKING = @GNULIB_UNISTD_H_NONBLOCKING@ GNULIB_UNISTD_H_SIGPIPE = @GNULIB_UNISTD_H_SIGPIPE@ GNULIB_UNLINK = @GNULIB_UNLINK@ GNULIB_UNLINKAT = @GNULIB_UNLINKAT@ GNULIB_UNLOCKPT = @GNULIB_UNLOCKPT@ GNULIB_UNSETENV = @GNULIB_UNSETENV@ GNULIB_USLEEP = @GNULIB_USLEEP@ GNULIB_UTIMENSAT = @GNULIB_UTIMENSAT@ GNULIB_VASPRINTF = @GNULIB_VASPRINTF@ GNULIB_VDPRINTF = @GNULIB_VDPRINTF@ GNULIB_VFPRINTF = @GNULIB_VFPRINTF@ GNULIB_VFPRINTF_POSIX = @GNULIB_VFPRINTF_POSIX@ GNULIB_VFSCANF = @GNULIB_VFSCANF@ GNULIB_VPRINTF = @GNULIB_VPRINTF@ GNULIB_VPRINTF_POSIX = @GNULIB_VPRINTF_POSIX@ GNULIB_VSCANF = @GNULIB_VSCANF@ GNULIB_VSNPRINTF = @GNULIB_VSNPRINTF@ GNULIB_VSPRINTF_POSIX = @GNULIB_VSPRINTF_POSIX@ GNULIB_WCPCPY = @GNULIB_WCPCPY@ GNULIB_WCPNCPY = @GNULIB_WCPNCPY@ GNULIB_WCRTOMB = @GNULIB_WCRTOMB@ GNULIB_WCSCASECMP = @GNULIB_WCSCASECMP@ GNULIB_WCSCAT = @GNULIB_WCSCAT@ GNULIB_WCSCHR = @GNULIB_WCSCHR@ GNULIB_WCSCMP = @GNULIB_WCSCMP@ GNULIB_WCSCOLL = @GNULIB_WCSCOLL@ GNULIB_WCSCPY = @GNULIB_WCSCPY@ GNULIB_WCSCSPN = @GNULIB_WCSCSPN@ GNULIB_WCSDUP = @GNULIB_WCSDUP@ GNULIB_WCSFTIME = @GNULIB_WCSFTIME@ GNULIB_WCSLEN = @GNULIB_WCSLEN@ GNULIB_WCSNCASECMP = @GNULIB_WCSNCASECMP@ GNULIB_WCSNCAT = @GNULIB_WCSNCAT@ GNULIB_WCSNCMP = @GNULIB_WCSNCMP@ GNULIB_WCSNCPY = @GNULIB_WCSNCPY@ GNULIB_WCSNLEN = @GNULIB_WCSNLEN@ GNULIB_WCSNRTOMBS = @GNULIB_WCSNRTOMBS@ GNULIB_WCSPBRK = @GNULIB_WCSPBRK@ GNULIB_WCSRCHR = @GNULIB_WCSRCHR@ GNULIB_WCSRTOMBS = @GNULIB_WCSRTOMBS@ GNULIB_WCSSPN = @GNULIB_WCSSPN@ GNULIB_WCSSTR = @GNULIB_WCSSTR@ GNULIB_WCSTOK = @GNULIB_WCSTOK@ GNULIB_WCSWIDTH = @GNULIB_WCSWIDTH@ GNULIB_WCSXFRM = @GNULIB_WCSXFRM@ GNULIB_WCTOB = @GNULIB_WCTOB@ GNULIB_WCTOMB = @GNULIB_WCTOMB@ GNULIB_WCTRANS = @GNULIB_WCTRANS@ GNULIB_WCTYPE = @GNULIB_WCTYPE@ GNULIB_WCWIDTH = @GNULIB_WCWIDTH@ GNULIB_WMEMCHR = @GNULIB_WMEMCHR@ GNULIB_WMEMCMP = @GNULIB_WMEMCMP@ GNULIB_WMEMCPY = @GNULIB_WMEMCPY@ GNULIB_WMEMMOVE = @GNULIB_WMEMMOVE@ GNULIB_WMEMSET = @GNULIB_WMEMSET@ GNULIB_WRITE = @GNULIB_WRITE@ GNULIB__EXIT = @GNULIB__EXIT@ GREP = @GREP@ GUIDEMESSAGE = @GUIDEMESSAGE@ HAVE_ACCEPT4 = @HAVE_ACCEPT4@ HAVE_ACOSF = @HAVE_ACOSF@ HAVE_ACOSL = @HAVE_ACOSL@ HAVE_ARPA_INET_H = @HAVE_ARPA_INET_H@ HAVE_ASINF = @HAVE_ASINF@ HAVE_ASINL = @HAVE_ASINL@ HAVE_ATAN2F = @HAVE_ATAN2F@ HAVE_ATANF = @HAVE_ATANF@ HAVE_ATANL = @HAVE_ATANL@ HAVE_ATOLL = @HAVE_ATOLL@ HAVE_BTOWC = @HAVE_BTOWC@ HAVE_C99_STDINT_H = @HAVE_C99_STDINT_H@ HAVE_CANONICALIZE_FILE_NAME = @HAVE_CANONICALIZE_FILE_NAME@ HAVE_CBRT = @HAVE_CBRT@ HAVE_CBRTF = @HAVE_CBRTF@ HAVE_CBRTL = @HAVE_CBRTL@ HAVE_CHOWN = @HAVE_CHOWN@ HAVE_COPYSIGN = @HAVE_COPYSIGN@ HAVE_COPYSIGNL = @HAVE_COPYSIGNL@ HAVE_COSF = @HAVE_COSF@ HAVE_COSHF = @HAVE_COSHF@ HAVE_COSL = @HAVE_COSL@ HAVE_CRTDEFS_H = @HAVE_CRTDEFS_H@ HAVE_DECL_ACOSL = @HAVE_DECL_ACOSL@ HAVE_DECL_ASINL = @HAVE_DECL_ASINL@ HAVE_DECL_ATANL = @HAVE_DECL_ATANL@ HAVE_DECL_CBRTF = @HAVE_DECL_CBRTF@ HAVE_DECL_CBRTL = @HAVE_DECL_CBRTL@ HAVE_DECL_CEILF = @HAVE_DECL_CEILF@ HAVE_DECL_CEILL = @HAVE_DECL_CEILL@ HAVE_DECL_COPYSIGNF = @HAVE_DECL_COPYSIGNF@ HAVE_DECL_COSL = @HAVE_DECL_COSL@ HAVE_DECL_ENVIRON = @HAVE_DECL_ENVIRON@ HAVE_DECL_EXP2 = @HAVE_DECL_EXP2@ HAVE_DECL_EXP2F = @HAVE_DECL_EXP2F@ HAVE_DECL_EXP2L = @HAVE_DECL_EXP2L@ HAVE_DECL_EXPL = @HAVE_DECL_EXPL@ HAVE_DECL_EXPM1L = @HAVE_DECL_EXPM1L@ HAVE_DECL_FCHDIR = @HAVE_DECL_FCHDIR@ HAVE_DECL_FDATASYNC = @HAVE_DECL_FDATASYNC@ HAVE_DECL_FLOORF = @HAVE_DECL_FLOORF@ HAVE_DECL_FLOORL = @HAVE_DECL_FLOORL@ HAVE_DECL_FPURGE = @HAVE_DECL_FPURGE@ HAVE_DECL_FREXPL = @HAVE_DECL_FREXPL@ HAVE_DECL_FSEEKO = @HAVE_DECL_FSEEKO@ HAVE_DECL_FTELLO = @HAVE_DECL_FTELLO@ HAVE_DECL_GETDELIM = @HAVE_DECL_GETDELIM@ HAVE_DECL_GETDOMAINNAME = @HAVE_DECL_GETDOMAINNAME@ HAVE_DECL_GETLINE = @HAVE_DECL_GETLINE@ HAVE_DECL_GETLOADAVG = @HAVE_DECL_GETLOADAVG@ HAVE_DECL_GETLOGIN = @HAVE_DECL_GETLOGIN@ HAVE_DECL_GETLOGIN_R = @HAVE_DECL_GETLOGIN_R@ HAVE_DECL_GETPAGESIZE = @HAVE_DECL_GETPAGESIZE@ HAVE_DECL_GETUSERSHELL = @HAVE_DECL_GETUSERSHELL@ HAVE_DECL_IMAXABS = @HAVE_DECL_IMAXABS@ HAVE_DECL_IMAXDIV = @HAVE_DECL_IMAXDIV@ HAVE_DECL_INET_NTOP = @HAVE_DECL_INET_NTOP@ HAVE_DECL_INET_PTON = @HAVE_DECL_INET_PTON@ HAVE_DECL_INITSTATE = @HAVE_DECL_INITSTATE@ HAVE_DECL_LDEXPL = @HAVE_DECL_LDEXPL@ HAVE_DECL_LOCALTIME_R = @HAVE_DECL_LOCALTIME_R@ HAVE_DECL_LOG10L = @HAVE_DECL_LOG10L@ HAVE_DECL_LOG2 = @HAVE_DECL_LOG2@ HAVE_DECL_LOG2F = @HAVE_DECL_LOG2F@ HAVE_DECL_LOG2L = @HAVE_DECL_LOG2L@ HAVE_DECL_LOGB = @HAVE_DECL_LOGB@ HAVE_DECL_LOGL = @HAVE_DECL_LOGL@ HAVE_DECL_MEMMEM = @HAVE_DECL_MEMMEM@ HAVE_DECL_MEMRCHR = @HAVE_DECL_MEMRCHR@ HAVE_DECL_OBSTACK_PRINTF = @HAVE_DECL_OBSTACK_PRINTF@ HAVE_DECL_REMAINDER = @HAVE_DECL_REMAINDER@ HAVE_DECL_REMAINDERL = @HAVE_DECL_REMAINDERL@ HAVE_DECL_RINTF = @HAVE_DECL_RINTF@ HAVE_DECL_ROUND = @HAVE_DECL_ROUND@ HAVE_DECL_ROUNDF = @HAVE_DECL_ROUNDF@ HAVE_DECL_ROUNDL = @HAVE_DECL_ROUNDL@ HAVE_DECL_SETENV = @HAVE_DECL_SETENV@ HAVE_DECL_SETHOSTNAME = @HAVE_DECL_SETHOSTNAME@ HAVE_DECL_SETSTATE = @HAVE_DECL_SETSTATE@ HAVE_DECL_SINL = @HAVE_DECL_SINL@ HAVE_DECL_SNPRINTF = @HAVE_DECL_SNPRINTF@ HAVE_DECL_SQRTL = @HAVE_DECL_SQRTL@ HAVE_DECL_STRDUP = @HAVE_DECL_STRDUP@ HAVE_DECL_STRERROR_R = @HAVE_DECL_STRERROR_R@ HAVE_DECL_STRNCASECMP = @HAVE_DECL_STRNCASECMP@ HAVE_DECL_STRNDUP = @HAVE_DECL_STRNDUP@ HAVE_DECL_STRNLEN = @HAVE_DECL_STRNLEN@ HAVE_DECL_STRSIGNAL = @HAVE_DECL_STRSIGNAL@ HAVE_DECL_STRTOIMAX = @HAVE_DECL_STRTOIMAX@ HAVE_DECL_STRTOK_R = @HAVE_DECL_STRTOK_R@ HAVE_DECL_STRTOUMAX = @HAVE_DECL_STRTOUMAX@ HAVE_DECL_TANL = @HAVE_DECL_TANL@ HAVE_DECL_TRUNC = @HAVE_DECL_TRUNC@ HAVE_DECL_TRUNCF = @HAVE_DECL_TRUNCF@ HAVE_DECL_TRUNCL = @HAVE_DECL_TRUNCL@ HAVE_DECL_TTYNAME_R = @HAVE_DECL_TTYNAME_R@ HAVE_DECL_UNSETENV = @HAVE_DECL_UNSETENV@ HAVE_DECL_VSNPRINTF = @HAVE_DECL_VSNPRINTF@ HAVE_DECL_WCTOB = @HAVE_DECL_WCTOB@ HAVE_DECL_WCWIDTH = @HAVE_DECL_WCWIDTH@ HAVE_DPRINTF = @HAVE_DPRINTF@ HAVE_DUP2 = @HAVE_DUP2@ HAVE_DUP3 = @HAVE_DUP3@ HAVE_DUPLOCALE = @HAVE_DUPLOCALE@ HAVE_EUIDACCESS = @HAVE_EUIDACCESS@ HAVE_EXPF = @HAVE_EXPF@ HAVE_EXPL = @HAVE_EXPL@ HAVE_EXPLICIT_BZERO = @HAVE_EXPLICIT_BZERO@ HAVE_EXPM1 = @HAVE_EXPM1@ HAVE_EXPM1F = @HAVE_EXPM1F@ HAVE_FABSF = @HAVE_FABSF@ HAVE_FABSL = @HAVE_FABSL@ HAVE_FACCESSAT = @HAVE_FACCESSAT@ HAVE_FCHDIR = @HAVE_FCHDIR@ HAVE_FCHMODAT = @HAVE_FCHMODAT@ HAVE_FCHOWNAT = @HAVE_FCHOWNAT@ HAVE_FCNTL = @HAVE_FCNTL@ HAVE_FDATASYNC = @HAVE_FDATASYNC@ HAVE_FEATURES_H = @HAVE_FEATURES_H@ HAVE_FFS = @HAVE_FFS@ HAVE_FFSL = @HAVE_FFSL@ HAVE_FFSLL = @HAVE_FFSLL@ HAVE_FMA = @HAVE_FMA@ HAVE_FMAF = @HAVE_FMAF@ HAVE_FMAL = @HAVE_FMAL@ HAVE_FMODF = @HAVE_FMODF@ HAVE_FMODL = @HAVE_FMODL@ HAVE_FREXPF = @HAVE_FREXPF@ HAVE_FSEEKO = @HAVE_FSEEKO@ HAVE_FSTATAT = @HAVE_FSTATAT@ HAVE_FSYNC = @HAVE_FSYNC@ HAVE_FTELLO = @HAVE_FTELLO@ HAVE_FTRUNCATE = @HAVE_FTRUNCATE@ HAVE_FUTIMENS = @HAVE_FUTIMENS@ HAVE_GETDTABLESIZE = @HAVE_GETDTABLESIZE@ HAVE_GETGROUPS = @HAVE_GETGROUPS@ HAVE_GETHOSTNAME = @HAVE_GETHOSTNAME@ HAVE_GETLOGIN = @HAVE_GETLOGIN@ HAVE_GETOPT_H = @HAVE_GETOPT_H@ HAVE_GETPAGESIZE = @HAVE_GETPAGESIZE@ HAVE_GETSUBOPT = @HAVE_GETSUBOPT@ HAVE_GETTIMEOFDAY = @HAVE_GETTIMEOFDAY@ HAVE_GRANTPT = @HAVE_GRANTPT@ HAVE_GROUP_MEMBER = @HAVE_GROUP_MEMBER@ HAVE_HYPOTF = @HAVE_HYPOTF@ HAVE_HYPOTL = @HAVE_HYPOTL@ HAVE_ILOGB = @HAVE_ILOGB@ HAVE_ILOGBF = @HAVE_ILOGBF@ HAVE_ILOGBL = @HAVE_ILOGBL@ HAVE_INTTYPES_H = @HAVE_INTTYPES_H@ HAVE_ISBLANK = @HAVE_ISBLANK@ HAVE_ISNAND = @HAVE_ISNAND@ HAVE_ISNANF = @HAVE_ISNANF@ HAVE_ISNANL = @HAVE_ISNANL@ HAVE_ISWBLANK = @HAVE_ISWBLANK@ HAVE_ISWCNTRL = @HAVE_ISWCNTRL@ HAVE_LANGINFO_CODESET = @HAVE_LANGINFO_CODESET@ HAVE_LANGINFO_ERA = @HAVE_LANGINFO_ERA@ HAVE_LANGINFO_H = @HAVE_LANGINFO_H@ HAVE_LANGINFO_T_FMT_AMPM = @HAVE_LANGINFO_T_FMT_AMPM@ HAVE_LANGINFO_YESEXPR = @HAVE_LANGINFO_YESEXPR@ HAVE_LCHMOD = @HAVE_LCHMOD@ HAVE_LCHOWN = @HAVE_LCHOWN@ HAVE_LDEXPF = @HAVE_LDEXPF@ HAVE_LIBGIT2 = @HAVE_LIBGIT2@ HAVE_LINK = @HAVE_LINK@ HAVE_LINKAT = @HAVE_LINKAT@ HAVE_LOG10F = @HAVE_LOG10F@ HAVE_LOG10L = @HAVE_LOG10L@ HAVE_LOG1P = @HAVE_LOG1P@ HAVE_LOG1PF = @HAVE_LOG1PF@ HAVE_LOG1PL = @HAVE_LOG1PL@ HAVE_LOGBF = @HAVE_LOGBF@ HAVE_LOGBL = @HAVE_LOGBL@ HAVE_LOGF = @HAVE_LOGF@ HAVE_LOGL = @HAVE_LOGL@ HAVE_LONG_LONG_INT = @HAVE_LONG_LONG_INT@ HAVE_LSTAT = @HAVE_LSTAT@ HAVE_MAX_ALIGN_T = @HAVE_MAX_ALIGN_T@ HAVE_MBRLEN = @HAVE_MBRLEN@ HAVE_MBRTOWC = @HAVE_MBRTOWC@ HAVE_MBSINIT = @HAVE_MBSINIT@ HAVE_MBSLEN = @HAVE_MBSLEN@ HAVE_MBSNRTOWCS = @HAVE_MBSNRTOWCS@ HAVE_MBSRTOWCS = @HAVE_MBSRTOWCS@ HAVE_MEMCHR = @HAVE_MEMCHR@ HAVE_MEMPCPY = @HAVE_MEMPCPY@ HAVE_MKDIRAT = @HAVE_MKDIRAT@ HAVE_MKDTEMP = @HAVE_MKDTEMP@ HAVE_MKFIFO = @HAVE_MKFIFO@ HAVE_MKFIFOAT = @HAVE_MKFIFOAT@ HAVE_MKNOD = @HAVE_MKNOD@ HAVE_MKNODAT = @HAVE_MKNODAT@ HAVE_MKOSTEMP = @HAVE_MKOSTEMP@ HAVE_MKOSTEMPS = @HAVE_MKOSTEMPS@ HAVE_MKSTEMP = @HAVE_MKSTEMP@ HAVE_MKSTEMPS = @HAVE_MKSTEMPS@ HAVE_MODFF = @HAVE_MODFF@ HAVE_MODFL = @HAVE_MODFL@ HAVE_MSVC_INVALID_PARAMETER_HANDLER = @HAVE_MSVC_INVALID_PARAMETER_HANDLER@ HAVE_NANOSLEEP = @HAVE_NANOSLEEP@ HAVE_NETINET_IN_H = @HAVE_NETINET_IN_H@ HAVE_NL_LANGINFO = @HAVE_NL_LANGINFO@ HAVE_OPENAT = @HAVE_OPENAT@ HAVE_OS_H = @HAVE_OS_H@ HAVE_PCLOSE = @HAVE_PCLOSE@ HAVE_PIPE = @HAVE_PIPE@ HAVE_PIPE2 = @HAVE_PIPE2@ HAVE_POPEN = @HAVE_POPEN@ HAVE_POSIX_OPENPT = @HAVE_POSIX_OPENPT@ HAVE_POSIX_SIGNALBLOCKING = @HAVE_POSIX_SIGNALBLOCKING@ HAVE_POWF = @HAVE_POWF@ HAVE_PREAD = @HAVE_PREAD@ HAVE_PSELECT = @HAVE_PSELECT@ HAVE_PTHREAD_BARRIER = @HAVE_PTHREAD_BARRIER@ HAVE_PTHREAD_SIGMASK = @HAVE_PTHREAD_SIGMASK@ HAVE_PTSNAME = @HAVE_PTSNAME@ HAVE_PTSNAME_R = @HAVE_PTSNAME_R@ HAVE_PWRITE = @HAVE_PWRITE@ HAVE_QSORT_R = @HAVE_QSORT_R@ HAVE_RAISE = @HAVE_RAISE@ HAVE_RANDOM = @HAVE_RANDOM@ HAVE_RANDOM_H = @HAVE_RANDOM_H@ HAVE_RANDOM_R = @HAVE_RANDOM_R@ HAVE_RAWMEMCHR = @HAVE_RAWMEMCHR@ HAVE_READLINK = @HAVE_READLINK@ HAVE_READLINKAT = @HAVE_READLINKAT@ HAVE_REALLOCARRAY = @HAVE_REALLOCARRAY@ HAVE_REALPATH = @HAVE_REALPATH@ HAVE_REMAINDER = @HAVE_REMAINDER@ HAVE_REMAINDERF = @HAVE_REMAINDERF@ HAVE_RENAMEAT = @HAVE_RENAMEAT@ HAVE_RINT = @HAVE_RINT@ HAVE_RINTL = @HAVE_RINTL@ HAVE_RPMATCH = @HAVE_RPMATCH@ HAVE_SAME_LONG_DOUBLE_AS_DOUBLE = @HAVE_SAME_LONG_DOUBLE_AS_DOUBLE@ HAVE_SA_FAMILY_T = @HAVE_SA_FAMILY_T@ HAVE_SECURE_GETENV = @HAVE_SECURE_GETENV@ HAVE_SETENV = @HAVE_SETENV@ HAVE_SETHOSTNAME = @HAVE_SETHOSTNAME@ HAVE_SIGACTION = @HAVE_SIGACTION@ HAVE_SIGHANDLER_T = @HAVE_SIGHANDLER_T@ HAVE_SIGINFO_T = @HAVE_SIGINFO_T@ HAVE_SIGNED_SIG_ATOMIC_T = @HAVE_SIGNED_SIG_ATOMIC_T@ HAVE_SIGNED_WCHAR_T = @HAVE_SIGNED_WCHAR_T@ HAVE_SIGNED_WINT_T = @HAVE_SIGNED_WINT_T@ HAVE_SIGSET_T = @HAVE_SIGSET_T@ HAVE_SINF = @HAVE_SINF@ HAVE_SINHF = @HAVE_SINHF@ HAVE_SINL = @HAVE_SINL@ HAVE_SLEEP = @HAVE_SLEEP@ HAVE_SQRTF = @HAVE_SQRTF@ HAVE_SQRTL = @HAVE_SQRTL@ HAVE_STDINT_H = @HAVE_STDINT_H@ HAVE_STPCPY = @HAVE_STPCPY@ HAVE_STPNCPY = @HAVE_STPNCPY@ HAVE_STRCASECMP = @HAVE_STRCASECMP@ HAVE_STRCASESTR = @HAVE_STRCASESTR@ HAVE_STRCHRNUL = @HAVE_STRCHRNUL@ HAVE_STRINGS_H = @HAVE_STRINGS_H@ HAVE_STRPBRK = @HAVE_STRPBRK@ HAVE_STRPTIME = @HAVE_STRPTIME@ HAVE_STRSEP = @HAVE_STRSEP@ HAVE_STRTOD = @HAVE_STRTOD@ HAVE_STRTOLL = @HAVE_STRTOLL@ HAVE_STRTOULL = @HAVE_STRTOULL@ HAVE_STRUCT_RANDOM_DATA = @HAVE_STRUCT_RANDOM_DATA@ HAVE_STRUCT_SIGACTION_SA_SIGACTION = @HAVE_STRUCT_SIGACTION_SA_SIGACTION@ HAVE_STRUCT_SOCKADDR_STORAGE = @HAVE_STRUCT_SOCKADDR_STORAGE@ HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY = @HAVE_STRUCT_SOCKADDR_STORAGE_SS_FAMILY@ HAVE_STRUCT_TIMEVAL = @HAVE_STRUCT_TIMEVAL@ HAVE_STRVERSCMP = @HAVE_STRVERSCMP@ HAVE_SYMLINK = @HAVE_SYMLINK@ HAVE_SYMLINKAT = @HAVE_SYMLINKAT@ HAVE_SYSEXITS_H = @HAVE_SYSEXITS_H@ HAVE_SYS_BITYPES_H = @HAVE_SYS_BITYPES_H@ HAVE_SYS_CDEFS_H = @HAVE_SYS_CDEFS_H@ HAVE_SYS_INTTYPES_H = @HAVE_SYS_INTTYPES_H@ HAVE_SYS_IOCTL_H = @HAVE_SYS_IOCTL_H@ HAVE_SYS_LOADAVG_H = @HAVE_SYS_LOADAVG_H@ HAVE_SYS_PARAM_H = @HAVE_SYS_PARAM_H@ HAVE_SYS_SELECT_H = @HAVE_SYS_SELECT_H@ HAVE_SYS_SOCKET_H = @HAVE_SYS_SOCKET_H@ HAVE_SYS_TIME_H = @HAVE_SYS_TIME_H@ HAVE_SYS_TYPES_H = @HAVE_SYS_TYPES_H@ HAVE_SYS_UIO_H = @HAVE_SYS_UIO_H@ HAVE_TANF = @HAVE_TANF@ HAVE_TANHF = @HAVE_TANHF@ HAVE_TANL = @HAVE_TANL@ HAVE_TIMEGM = @HAVE_TIMEGM@ HAVE_TIMEZONE_T = @HAVE_TIMEZONE_T@ HAVE_TRUNCATE = @HAVE_TRUNCATE@ HAVE_TYPE_VOLATILE_SIG_ATOMIC_T = @HAVE_TYPE_VOLATILE_SIG_ATOMIC_T@ HAVE_TZSET = @HAVE_TZSET@ HAVE_UNISTD_H = @HAVE_UNISTD_H@ HAVE_UNLINKAT = @HAVE_UNLINKAT@ HAVE_UNLOCKPT = @HAVE_UNLOCKPT@ HAVE_UNSIGNED_LONG_LONG_INT = @HAVE_UNSIGNED_LONG_LONG_INT@ HAVE_USLEEP = @HAVE_USLEEP@ HAVE_UTIMENSAT = @HAVE_UTIMENSAT@ HAVE_VASPRINTF = @HAVE_VASPRINTF@ HAVE_VDPRINTF = @HAVE_VDPRINTF@ HAVE_WCHAR_H = @HAVE_WCHAR_H@ HAVE_WCHAR_T = @HAVE_WCHAR_T@ HAVE_WCPCPY = @HAVE_WCPCPY@ HAVE_WCPNCPY = @HAVE_WCPNCPY@ HAVE_WCRTOMB = @HAVE_WCRTOMB@ HAVE_WCSCASECMP = @HAVE_WCSCASECMP@ HAVE_WCSCAT = @HAVE_WCSCAT@ HAVE_WCSCHR = @HAVE_WCSCHR@ HAVE_WCSCMP = @HAVE_WCSCMP@ HAVE_WCSCOLL = @HAVE_WCSCOLL@ HAVE_WCSCPY = @HAVE_WCSCPY@ HAVE_WCSCSPN = @HAVE_WCSCSPN@ HAVE_WCSDUP = @HAVE_WCSDUP@ HAVE_WCSFTIME = @HAVE_WCSFTIME@ HAVE_WCSLEN = @HAVE_WCSLEN@ HAVE_WCSLIB_VERSION = @HAVE_WCSLIB_VERSION@ HAVE_WCSNCASECMP = @HAVE_WCSNCASECMP@ HAVE_WCSNCAT = @HAVE_WCSNCAT@ HAVE_WCSNCMP = @HAVE_WCSNCMP@ HAVE_WCSNCPY = @HAVE_WCSNCPY@ HAVE_WCSNLEN = @HAVE_WCSNLEN@ HAVE_WCSNRTOMBS = @HAVE_WCSNRTOMBS@ HAVE_WCSPBRK = @HAVE_WCSPBRK@ HAVE_WCSRCHR = @HAVE_WCSRCHR@ HAVE_WCSRTOMBS = @HAVE_WCSRTOMBS@ HAVE_WCSSPN = @HAVE_WCSSPN@ HAVE_WCSSTR = @HAVE_WCSSTR@ HAVE_WCSTOK = @HAVE_WCSTOK@ HAVE_WCSWIDTH = @HAVE_WCSWIDTH@ HAVE_WCSXFRM = @HAVE_WCSXFRM@ HAVE_WCTRANS_T = @HAVE_WCTRANS_T@ HAVE_WCTYPE_H = @HAVE_WCTYPE_H@ HAVE_WCTYPE_T = @HAVE_WCTYPE_T@ HAVE_WINSOCK2_H = @HAVE_WINSOCK2_H@ HAVE_WINT_T = @HAVE_WINT_T@ HAVE_WMEMCHR = @HAVE_WMEMCHR@ HAVE_WMEMCMP = @HAVE_WMEMCMP@ HAVE_WMEMCPY = @HAVE_WMEMCPY@ HAVE_WMEMMOVE = @HAVE_WMEMMOVE@ HAVE_WMEMSET = @HAVE_WMEMSET@ HAVE_WS2TCPIP_H = @HAVE_WS2TCPIP_H@ HAVE_XLOCALE_H = @HAVE_XLOCALE_H@ HAVE__BOOL = @HAVE__BOOL@ HAVE__EXIT = @HAVE__EXIT@ HOST_CPU = @HOST_CPU@ HOST_CPU_C_ABI = @HOST_CPU_C_ABI@ INCLUDE_NEXT = @INCLUDE_NEXT@ INCLUDE_NEXT_AS_FIRST_DIRECTIVE = @INCLUDE_NEXT_AS_FIRST_DIRECTIVE@ INET_PTON_LIB = @INET_PTON_LIB@ INSTALL = @INSTALL@ INSTALL_DATA = @INSTALL_DATA@ INSTALL_PROGRAM = @INSTALL_PROGRAM@ INSTALL_SCRIPT = @INSTALL_SCRIPT@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@ INT32_MAX_LT_INTMAX_MAX = @INT32_MAX_LT_INTMAX_MAX@ INT64_MAX_EQ_LONG_MAX = @INT64_MAX_EQ_LONG_MAX@ INTL_MACOSX_LIBS = @INTL_MACOSX_LIBS@ LD = @LD@ LDFLAGS = @LDFLAGS@ LIBINTL = @LIBINTL@ LIBMULTITHREAD = @LIBMULTITHREAD@ LIBOBJS = @LIBOBJS@ LIBPTH = @LIBPTH@ LIBPTH_PREFIX = @LIBPTH_PREFIX@ LIBS = @LIBS@ LIBSOCKET = @LIBSOCKET@ LIBTESTS_LIBDEPS = @LIBTESTS_LIBDEPS@ LIBTHREAD = @LIBTHREAD@ LIBTOOL = @LIBTOOL@ LIBUNISTRING_UNITYPES_H = @LIBUNISTRING_UNITYPES_H@ LIBUNISTRING_UNIWIDTH_H = @LIBUNISTRING_UNIWIDTH_H@ LIB_NANOSLEEP = @LIB_NANOSLEEP@ LIB_PTHREAD_SIGMASK = @LIB_PTHREAD_SIGMASK@ LIB_SELECT = @LIB_SELECT@ LIMITS_H = @LIMITS_H@ LIPO = @LIPO@ LN_S = @LN_S@ LOCALCHARSET_TESTS_ENVIRONMENT = @LOCALCHARSET_TESTS_ENVIRONMENT@ LOCALE_FR = @LOCALE_FR@ LOCALE_FR_UTF8 = @LOCALE_FR_UTF8@ LOCALE_JA = @LOCALE_JA@ LOCALE_TR_UTF8 = @LOCALE_TR_UTF8@ LOCALE_ZH_CN = @LOCALE_ZH_CN@ LTALLOCA = @LTALLOCA@ LTLIBINTL = @LTLIBINTL@ LTLIBMULTITHREAD = @LTLIBMULTITHREAD@ LTLIBOBJS = @LTLIBOBJS@ LTLIBPTH = @LTLIBPTH@ LTLIBTHREAD = @LTLIBTHREAD@ LT_SYS_LIBRARY_PATH = @LT_SYS_LIBRARY_PATH@ MAKEINFO = @MAKEINFO@ MANIFEST_TOOL = @MANIFEST_TOOL@ MKDIR_P = @MKDIR_P@ NETINET_IN_H = @NETINET_IN_H@ NEXT_ARPA_INET_H = @NEXT_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H = @NEXT_AS_FIRST_DIRECTIVE_ARPA_INET_H@ NEXT_AS_FIRST_DIRECTIVE_CTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_CTYPE_H@ NEXT_AS_FIRST_DIRECTIVE_ERRNO_H = @NEXT_AS_FIRST_DIRECTIVE_ERRNO_H@ NEXT_AS_FIRST_DIRECTIVE_FCNTL_H = @NEXT_AS_FIRST_DIRECTIVE_FCNTL_H@ NEXT_AS_FIRST_DIRECTIVE_FLOAT_H = @NEXT_AS_FIRST_DIRECTIVE_FLOAT_H@ NEXT_AS_FIRST_DIRECTIVE_GETOPT_H = @NEXT_AS_FIRST_DIRECTIVE_GETOPT_H@ NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H = @NEXT_AS_FIRST_DIRECTIVE_INTTYPES_H@ NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H = @NEXT_AS_FIRST_DIRECTIVE_LANGINFO_H@ NEXT_AS_FIRST_DIRECTIVE_LIMITS_H = @NEXT_AS_FIRST_DIRECTIVE_LIMITS_H@ NEXT_AS_FIRST_DIRECTIVE_LOCALE_H = @NEXT_AS_FIRST_DIRECTIVE_LOCALE_H@ NEXT_AS_FIRST_DIRECTIVE_MATH_H = @NEXT_AS_FIRST_DIRECTIVE_MATH_H@ NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H = @NEXT_AS_FIRST_DIRECTIVE_NETINET_IN_H@ NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H = @NEXT_AS_FIRST_DIRECTIVE_SIGNAL_H@ NEXT_AS_FIRST_DIRECTIVE_STDDEF_H = @NEXT_AS_FIRST_DIRECTIVE_STDDEF_H@ NEXT_AS_FIRST_DIRECTIVE_STDINT_H = @NEXT_AS_FIRST_DIRECTIVE_STDINT_H@ NEXT_AS_FIRST_DIRECTIVE_STDIO_H = @NEXT_AS_FIRST_DIRECTIVE_STDIO_H@ NEXT_AS_FIRST_DIRECTIVE_STDLIB_H = @NEXT_AS_FIRST_DIRECTIVE_STDLIB_H@ NEXT_AS_FIRST_DIRECTIVE_STRINGS_H = @NEXT_AS_FIRST_DIRECTIVE_STRINGS_H@ NEXT_AS_FIRST_DIRECTIVE_STRING_H = @NEXT_AS_FIRST_DIRECTIVE_STRING_H@ NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H = @NEXT_AS_FIRST_DIRECTIVE_SYSEXITS_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_IOCTL_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SELECT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_SOCKET_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_STAT_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_TYPES_H@ NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H = @NEXT_AS_FIRST_DIRECTIVE_SYS_UIO_H@ NEXT_AS_FIRST_DIRECTIVE_TIME_H = @NEXT_AS_FIRST_DIRECTIVE_TIME_H@ NEXT_AS_FIRST_DIRECTIVE_UNISTD_H = @NEXT_AS_FIRST_DIRECTIVE_UNISTD_H@ NEXT_AS_FIRST_DIRECTIVE_WCHAR_H = @NEXT_AS_FIRST_DIRECTIVE_WCHAR_H@ NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H = @NEXT_AS_FIRST_DIRECTIVE_WCTYPE_H@ NEXT_CTYPE_H = @NEXT_CTYPE_H@ NEXT_ERRNO_H = @NEXT_ERRNO_H@ NEXT_FCNTL_H = @NEXT_FCNTL_H@ NEXT_FLOAT_H = @NEXT_FLOAT_H@ NEXT_GETOPT_H = @NEXT_GETOPT_H@ NEXT_INTTYPES_H = @NEXT_INTTYPES_H@ NEXT_LANGINFO_H = @NEXT_LANGINFO_H@ NEXT_LIMITS_H = @NEXT_LIMITS_H@ NEXT_LOCALE_H = @NEXT_LOCALE_H@ NEXT_MATH_H = @NEXT_MATH_H@ NEXT_NETINET_IN_H = @NEXT_NETINET_IN_H@ NEXT_SIGNAL_H = @NEXT_SIGNAL_H@ NEXT_STDDEF_H = @NEXT_STDDEF_H@ NEXT_STDINT_H = @NEXT_STDINT_H@ NEXT_STDIO_H = @NEXT_STDIO_H@ NEXT_STDLIB_H = @NEXT_STDLIB_H@ NEXT_STRINGS_H = @NEXT_STRINGS_H@ NEXT_STRING_H = @NEXT_STRING_H@ NEXT_SYSEXITS_H = @NEXT_SYSEXITS_H@ NEXT_SYS_IOCTL_H = @NEXT_SYS_IOCTL_H@ NEXT_SYS_SELECT_H = @NEXT_SYS_SELECT_H@ NEXT_SYS_SOCKET_H = @NEXT_SYS_SOCKET_H@ NEXT_SYS_STAT_H = @NEXT_SYS_STAT_H@ NEXT_SYS_TIME_H = @NEXT_SYS_TIME_H@ NEXT_SYS_TYPES_H = @NEXT_SYS_TYPES_H@ NEXT_SYS_UIO_H = @NEXT_SYS_UIO_H@ NEXT_TIME_H = @NEXT_TIME_H@ NEXT_UNISTD_H = @NEXT_UNISTD_H@ NEXT_WCHAR_H = @NEXT_WCHAR_H@ NEXT_WCTYPE_H = @NEXT_WCTYPE_H@ NM = @NM@ NMEDIT = @NMEDIT@ OBJDUMP = @OBJDUMP@ OBJEXT = @OBJEXT@ OTOOL = @OTOOL@ OTOOL64 = @OTOOL64@ PACKAGE = @PACKAGE@ PACKAGE_BUGREPORT = @PACKAGE_BUGREPORT@ PACKAGE_NAME = @PACKAGE_NAME@ PACKAGE_STRING = @PACKAGE_STRING@ PACKAGE_TARNAME = @PACKAGE_TARNAME@ PACKAGE_URL = @PACKAGE_URL@ PACKAGE_VERSION = @PACKAGE_VERSION@ PATH_SEPARATOR = @PATH_SEPARATOR@ PRAGMA_COLUMNS = @PRAGMA_COLUMNS@ PRAGMA_SYSTEM_HEADER = @PRAGMA_SYSTEM_HEADER@ PRIPTR_PREFIX = @PRIPTR_PREFIX@ PRI_MACROS_BROKEN = @PRI_MACROS_BROKEN@ PTHREAD_CC = @PTHREAD_CC@ PTHREAD_CFLAGS = @PTHREAD_CFLAGS@ PTHREAD_H_DEFINES_STRUCT_TIMESPEC = @PTHREAD_H_DEFINES_STRUCT_TIMESPEC@ PTHREAD_LIBS = @PTHREAD_LIBS@ PTRDIFF_T_SUFFIX = @PTRDIFF_T_SUFFIX@ RANLIB = @RANLIB@ REPLACE_ACOSF = @REPLACE_ACOSF@ REPLACE_ASINF = @REPLACE_ASINF@ REPLACE_ATAN2F = @REPLACE_ATAN2F@ REPLACE_ATANF = @REPLACE_ATANF@ REPLACE_BTOWC = @REPLACE_BTOWC@ REPLACE_CALLOC = @REPLACE_CALLOC@ REPLACE_CANONICALIZE_FILE_NAME = @REPLACE_CANONICALIZE_FILE_NAME@ REPLACE_CBRTF = @REPLACE_CBRTF@ REPLACE_CBRTL = @REPLACE_CBRTL@ REPLACE_CEIL = @REPLACE_CEIL@ REPLACE_CEILF = @REPLACE_CEILF@ REPLACE_CEILL = @REPLACE_CEILL@ REPLACE_CHOWN = @REPLACE_CHOWN@ REPLACE_CLOSE = @REPLACE_CLOSE@ REPLACE_COSF = @REPLACE_COSF@ REPLACE_COSHF = @REPLACE_COSHF@ REPLACE_CTIME = @REPLACE_CTIME@ REPLACE_DPRINTF = @REPLACE_DPRINTF@ REPLACE_DUP = @REPLACE_DUP@ REPLACE_DUP2 = @REPLACE_DUP2@ REPLACE_DUPLOCALE = @REPLACE_DUPLOCALE@ REPLACE_EXP2 = @REPLACE_EXP2@ REPLACE_EXP2L = @REPLACE_EXP2L@ REPLACE_EXPF = @REPLACE_EXPF@ REPLACE_EXPM1 = @REPLACE_EXPM1@ REPLACE_EXPM1F = @REPLACE_EXPM1F@ REPLACE_FABSL = @REPLACE_FABSL@ REPLACE_FACCESSAT = @REPLACE_FACCESSAT@ REPLACE_FCHOWNAT = @REPLACE_FCHOWNAT@ REPLACE_FCLOSE = @REPLACE_FCLOSE@ REPLACE_FCNTL = @REPLACE_FCNTL@ REPLACE_FDOPEN = @REPLACE_FDOPEN@ REPLACE_FFLUSH = @REPLACE_FFLUSH@ REPLACE_FLOOR = @REPLACE_FLOOR@ REPLACE_FLOORF = @REPLACE_FLOORF@ REPLACE_FLOORL = @REPLACE_FLOORL@ REPLACE_FMA = @REPLACE_FMA@ REPLACE_FMAF = @REPLACE_FMAF@ REPLACE_FMAL = @REPLACE_FMAL@ REPLACE_FMOD = @REPLACE_FMOD@ REPLACE_FMODF = @REPLACE_FMODF@ REPLACE_FMODL = @REPLACE_FMODL@ REPLACE_FOPEN = @REPLACE_FOPEN@ REPLACE_FPRINTF = @REPLACE_FPRINTF@ REPLACE_FPURGE = @REPLACE_FPURGE@ REPLACE_FREOPEN = @REPLACE_FREOPEN@ REPLACE_FREXP = @REPLACE_FREXP@ REPLACE_FREXPF = @REPLACE_FREXPF@ REPLACE_FREXPL = @REPLACE_FREXPL@ REPLACE_FSEEK = @REPLACE_FSEEK@ REPLACE_FSEEKO = @REPLACE_FSEEKO@ REPLACE_FSTAT = @REPLACE_FSTAT@ REPLACE_FSTATAT = @REPLACE_FSTATAT@ REPLACE_FTELL = @REPLACE_FTELL@ REPLACE_FTELLO = @REPLACE_FTELLO@ REPLACE_FTRUNCATE = @REPLACE_FTRUNCATE@ REPLACE_FUTIMENS = @REPLACE_FUTIMENS@ REPLACE_GETCWD = @REPLACE_GETCWD@ REPLACE_GETDELIM = @REPLACE_GETDELIM@ REPLACE_GETDOMAINNAME = @REPLACE_GETDOMAINNAME@ REPLACE_GETDTABLESIZE = @REPLACE_GETDTABLESIZE@ REPLACE_GETGROUPS = @REPLACE_GETGROUPS@ REPLACE_GETLINE = @REPLACE_GETLINE@ REPLACE_GETLOGIN_R = @REPLACE_GETLOGIN_R@ REPLACE_GETPAGESIZE = @REPLACE_GETPAGESIZE@ REPLACE_GETTIMEOFDAY = @REPLACE_GETTIMEOFDAY@ REPLACE_GMTIME = @REPLACE_GMTIME@ REPLACE_HUGE_VAL = @REPLACE_HUGE_VAL@ REPLACE_HYPOT = @REPLACE_HYPOT@ REPLACE_HYPOTF = @REPLACE_HYPOTF@ REPLACE_HYPOTL = @REPLACE_HYPOTL@ REPLACE_ILOGB = @REPLACE_ILOGB@ REPLACE_ILOGBF = @REPLACE_ILOGBF@ REPLACE_ILOGBL = @REPLACE_ILOGBL@ REPLACE_INET_NTOP = @REPLACE_INET_NTOP@ REPLACE_INET_PTON = @REPLACE_INET_PTON@ REPLACE_IOCTL = @REPLACE_IOCTL@ REPLACE_ISATTY = @REPLACE_ISATTY@ REPLACE_ISFINITE = @REPLACE_ISFINITE@ REPLACE_ISINF = @REPLACE_ISINF@ REPLACE_ISNAN = @REPLACE_ISNAN@ REPLACE_ISWBLANK = @REPLACE_ISWBLANK@ REPLACE_ISWCNTRL = @REPLACE_ISWCNTRL@ REPLACE_ITOLD = @REPLACE_ITOLD@ REPLACE_LCHOWN = @REPLACE_LCHOWN@ REPLACE_LDEXPL = @REPLACE_LDEXPL@ REPLACE_LINK = @REPLACE_LINK@ REPLACE_LINKAT = @REPLACE_LINKAT@ REPLACE_LOCALECONV = @REPLACE_LOCALECONV@ REPLACE_LOCALTIME = @REPLACE_LOCALTIME@ REPLACE_LOCALTIME_R = @REPLACE_LOCALTIME_R@ REPLACE_LOG = @REPLACE_LOG@ REPLACE_LOG10 = @REPLACE_LOG10@ REPLACE_LOG10F = @REPLACE_LOG10F@ REPLACE_LOG10L = @REPLACE_LOG10L@ REPLACE_LOG1P = @REPLACE_LOG1P@ REPLACE_LOG1PF = @REPLACE_LOG1PF@ REPLACE_LOG1PL = @REPLACE_LOG1PL@ REPLACE_LOG2 = @REPLACE_LOG2@ REPLACE_LOG2F = @REPLACE_LOG2F@ REPLACE_LOG2L = @REPLACE_LOG2L@ REPLACE_LOGB = @REPLACE_LOGB@ REPLACE_LOGBF = 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installcheck-am \ installdirs maintainer-clean maintainer-clean-generic \ mostlyclean mostlyclean-compile mostlyclean-generic \ mostlyclean-libtool pdf pdf-am ps ps-am tags tags-am uninstall \ uninstall-am uninstall-binPROGRAMS uninstall-dist_sysconfDATA .PRECIOUS: Makefile # Tell versions [3.59,3.63) of GNU make to not export all variables. # Otherwise a system limit (for SysV at least) may be exceeded. .NOEXPORT: �����������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/astarithmetic.conf������������������������������������������������������0000644�0001750�0001750�00000001611�13121462410�016543� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default parameters (System) for Arithmetic. # Arithmetic is part of GNU Astronomy Utitlies. # # Use the long option name of each parameter followed by a value. The name # and value should be separated by atleast one white-space character (for # example ` '[space], or tab). Lines starting with `#' are ignored. # # For more information, please run these commands: # # $ astarithmetic --help # Full list of options, short doc. # $ astarithmetic -P # Print all options and used values. # $ info astarithmetic # All options and input/output. # $ info gnuastro "Configuration files" # How to use configuration files. # # Copying and distribution of this file, with or without modification, are # permitted in any medium without royalty provided the copyright notice and # this notice are preserved. This file is offered as-is, without any # warranty. �����������������������������������������������������������������������������������������������������������������������gnuastro-0.5/bin/arithmetic/Makefile.am�������������������������������������������������������������0000644�0001750�0001750�00000002644�13121462410�015076� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������## Process this file with automake to produce Makefile.inx ## ## Original author: ## Mohammad Akhlaghi <akhlaghi@gnu.org> ## Contributing author(s): ## Copyright (C) 2015, Free Software Foundation, Inc. ## ## Gnuastro is free software: you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation, either version 3 of the License, or ## (at your option) any later version. ## ## Gnuastro is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Gnuastro. If not, see <http://www.gnu.org/licenses/>. ## Pre-processer flags (for Gnulib's headers). Recall that the compiled ## Gnulib library was statically linked to (copied in) Gnuastro's library. AM_CPPFLAGS = -I\$(top_srcdir)/bootstrapped/lib ## Program definition (name, linking, sources and headers) bin_PROGRAMS = astarithmetic astarithmetic_LDADD = -lgnuastro astarithmetic_SOURCES = main.c ui.c arithmetic.c operands.c EXTRA_DIST = main.h authors-cite.h args.h ui.h arithmetic.h operands.h ## The configuration file (distribute and install). ## NOTE: the man page is created in doc/Makefile.am dist_sysconf_DATA = astarithmetic.conf ��������������������������������������������������������������������������������������������gnuastro-0.5/bin/gnuastro.conf����������������������������������������������������������������������0000644�0001750�0001750�00000001755�13142046236�013433� �����������������������������������������������������������������������������������������������������������������������������������������������������������������������������0000000�0000000������������������������������������������������������������������������������������������������������������������������������������������������������������������������# Default values for the common options to all the programs in GNU # Astronomy Utitlies. # # Use the long option name of each paramter followed by # a value. The name and value should be separated by # atleast one of the following charaacters: # space, `,`, `=` or `:` # # Run with `--help` option or read the manual for a full # explanation of what each option means. # # NOTE I: All counting is from zero, not one. # NOTE II: Lines starting with `#` are ignored. # # Copying and distribution of this file, with or without modification, # are permitted in any medium without royalty provided the copyright # notice and this notice are preserved. This file is offered as-is, # without any warranty. # Input: hdu 1 ignorecase 1 searchin name # Tessellation tilesize 50,50 numchannels 1,1 remainderfrac 0.1 workoverch 0 interpnumngb 9 interponlyblank 0 # Output: tableformat fits-binary # Operating mode minmapsize 1000000000����������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������������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